Presentation type:
NP – Nonlinear Processes in Geosciences

EGU26-1503 | Orals | MAL24-NP | Lewis Fry Richardson Medal Lecture

On the Origins of Randomness 

Anastasios Tsonis

This presentation discusses the definition of randomness, the sources of randomness in the physical system (the Universe) as well as in the formal mathematical system. I discuss how randomness, through nonlinearity and chaos, the second law of thermodynamics, the quantum mechanical character of small scales, and stochasticity, is an intrinsic property of nature. I then move to our mathematical system and show that even in this formal system we cannot do away with randomness, and that the randomness in the physical world is consistent with the origins of randomness suggested from the study of mathematical systems. Many examples are presented ranging from pure mathematical processes, to natural processes, to social processes, and to life in general, which clearly demonstrate how the combination of rules and randomness produces and explains the world we live in. Finally, a possible explanation is provided as to why rules and randomness cannot exist by themselves but instead, they have to coexist.

 

How to cite: Tsonis, A.: On the Origins of Randomness, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1503, https://doi.org/10.5194/egusphere-egu26-1503, 2026.

EGU26-21589 | ECS | Orals | MAL24-NP | Arne Richter Award for Outstanding ECS Lecture

Is it possible to have confidence in climate information with structurally uncertain models? 

Francisco de Melo Viríssimo

Climate models, in the form of Earth System Models (ESMs), are central to both climate science and climate-informed decision-making. Technically, they are complex, nonautonomous, and chaotic mathematical and computational representations of the Earth’s interacting “spheres”, including the atmosphere, oceans, cryosphere and biosphere. In practice, they are widely used to produce conditional projections of future climate under prescribed forcing and emissions scenarios - and remain the only tools capable of doing so within a physically consistent framework. However, despite their indispensable role, the interpretation of ESM outputs is fundamentally constrained by multiple sources of uncertainty, normally grouped as internal climate variability, uncertainty in future forcing scenarios, and uncertainty arising from model formulation.

While internal variability and scenario uncertainty have traditionally received most attention, attempts to partition uncertainty (e.g. [1]) have shown that it is actually the latter, model uncertainty, which is responsible for most uncertainty in climate projections. But despite its relevance, model uncertainty is frequently treated only implicitly, commonly subsumed under the broad label of “structural uncertainty”, with limited clarity regarding its definition or impact. This raises several unresolved questions of direct relevance to both modelling and decision-making efforts: what constitutes structural uncertainty in contemporary ESMs, how does it propagate through ensembles and projections, and how does it affect downstream socio-economic impact assessments and climate risk analyses? 

In this presentation, I will discuss these questions by reviewing recent advances in the characterisation and interpretation of model uncertainty (including results from my collaborators and myself, e.g. [2-4]) and examining their implications for the use of climate projections in scientific inference and decision-making. I conclude by identifying key conceptual and methodological gaps that must be addressed to improve confidence in climate information under persistent structural uncertainty.

With many and wholehearted thanks to all my collaborators, mentors, friends, colleagues, students and funders who made the journey to this award possible.

References:

[1] Lehner, F., Deser, C., Maher, N., Marotzke, J., Fischer, E. M., Brunner, L., Knutti, R., and Hawkins, E. (2020): Partitioning climate projection uncertainty with multiple large ensembles and CMIP5/6. Earth System Dynamics, 11, 491–508. https://doi.org/10.5194/esd-11-491-2020

[2] de Melo Viríssimo, F., Stainforth, D. A., and Bröcker, J. (2024): The evolution of a non-autonomous chaotic system under non-periodic forcing: A climate change example. Chaos, 34, 013136. https://doi.org/10.1063/5.0180870

[3] Martin, A. P., Bahamondes Dominguez, A., Baker, C. A., Baumas, C. M. J., Bisson, K. M., Cavan, E., Freilich, M., Galbraith, E., Galí, M., Henson, S., Kvale, K. F., Lemmen, C., Luo, J. Y., McMonagle, H., de Melo Viríssimo, F., Möller, K. O., Richon, C., Suresh, I., Wilson, J. D., Woodstock, M. S., and Yool, A. (2024): When to add a new process to a model – and when not: A marine biogeochemical perspective. Ecological Modelling, 498, 110870. https://doi.org/10.1016/j.ecolmodel.2024.110870

[4] de Melo Viríssimo, F., and Stainforth, D. A. (2025): Micro- and Macroparametric Uncertainty in Climate Change Prediction: A Large Ensemble Perspective. Bulletin of the American Meteorological Society, 106, E1319–E1341. https://doi.org/10.1175/BAMS-D-24-0064.1

How to cite: de Melo Viríssimo, F.: Is it possible to have confidence in climate information with structurally uncertain models?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21589, https://doi.org/10.5194/egusphere-egu26-21589, 2026.

EGU26-5340 | ECS | Posters virtual | VPS21

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

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

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

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

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

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

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

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

 

 

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

EGU26-11154 | ECS | Posters virtual | VPS21

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

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

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

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

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

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

EGU26-13270 | Posters virtual | VPS21

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

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

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

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

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

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

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

EGU26-13783 | Posters virtual | VPS21

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

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

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

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

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

EGU26-13852 | ECS | Posters virtual | VPS21

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

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

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

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

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

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

EGU26-19784 | Posters virtual | VPS21

Operationalising Semantic Interoperability for Cross-domain Discovery with LUMIS 

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

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

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

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

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

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

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

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

EGU26-20391 | Posters virtual | VPS21

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

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

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

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

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

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

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

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

EGU26-21793 | Posters virtual | VPS21

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

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

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

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

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

EGU26-21965 | Posters virtual | VPS21

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

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

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

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

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

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

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

EGU26-22084 | ECS | Posters virtual | VPS21

Monitoring Groundwater Quality and Improvement in the Kima Area, Aswan 

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

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

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

EGU26-3080 | ECS | Posters virtual | VPS22

Multibranch Adaptive Feature Fusion for Hyperspectral Image Classification 

Chen Li and Baoyu Du

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

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

EGU26-3363 | ECS | Posters virtual | VPS22

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

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

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

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

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

EGU26-3619 | ECS | Posters virtual | VPS22

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

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

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

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

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

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

EGU26-6022 | ECS | Posters virtual | VPS22

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

Harold Buitrago, Juan Contreras, and Florian Neumann

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

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

EGU26-6232 | Posters virtual | VPS22

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

Shaomeng Li, Allison Baker, and Lulin Xue

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

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

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

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

 

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

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

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

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

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

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

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

EGU26-11945 | Posters virtual | VPS22

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

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

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

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

EGU26-13611 | ECS | Posters virtual | VPS22

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

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

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

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

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

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

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

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

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

EGU26-4129 | ECS | Posters virtual | VPS23

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

Abhiram Doddi, David Fritts, and Thomas Lund

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

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

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

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

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

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

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

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

EGU26-4184 | ECS | Posters virtual | VPS23

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

Arun kumar Beerkur and Hussain Palagiri

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

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

EGU26-4200 | ECS | Posters virtual | VPS23

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

Karmishtha Karmishtha, Rajesh Kumar Behera, and Gopal Das Singhal

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

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

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

EGU26-4951 | ECS | Posters virtual | VPS23

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

Anil Kumar, Ellora Padhi, and Surendra Kumar Mishra

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

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

EGU26-5098 | ECS | Posters virtual | VPS23

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

Pavithra Belluti Nanjundagowda and Vamsi Krishna Vema

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

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

EGU26-5765 | ECS | Posters virtual | VPS23

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

Kuan Jiang, Chengzhi Qi, and Xiaoyue Hu

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

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

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

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

EGU26-8596 | ECS | Posters virtual | VPS23

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

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

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

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

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

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

EGU26-8813 | ECS | Posters virtual | VPS23

Assessment of Partial Blockage in Urban Drains for Flood Risk Reduction  

Aayusha Kumari Mishra, Hemant Kumar, and Rajendran Vinnarasi

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

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

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

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

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

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

EGU26-8985 | ECS | Posters virtual | VPS23

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

Maoqian Zhang, Arcady Dyskin, and Elena Pasternak

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

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

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

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

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

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

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

EGU26-13831 | ECS | Posters virtual | VPS23

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

Damodar Sharma, Surendra Kumar Mishra, and Rajendra Prasad Pandey

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

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

EGU26-15102 | Posters virtual | VPS23

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

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

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

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

EGU26-16403 | ECS | Posters virtual | VPS23

Assessing the Impact of Digital Elevation Model Selection on Hydrological Predictions 

Prashant Prashant, Surendra Kumar Mishra, and Anil Kumar Lohani

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

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

EGU26-18007 | ECS | Posters virtual | VPS23

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

Jyothi Banothu and Kamalini Devi

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

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

EGU26-18481 | ECS | Posters virtual | VPS23

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

Pushparaj Singh, Rahul Deopa, and Mohit Prakash Mohanty

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

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

EGU26-18820 | ECS | Posters virtual | VPS23

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

Adrian van Kan, Jeffrey Weiss, and Edgar Knobloch

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

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

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

EGU26-19471 | ECS | Posters virtual | VPS23

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

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

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

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

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

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

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

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

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

EGU26-21173 | Posters virtual | VPS23

Global Hot Spots of Climate Extremes from Composite Hazard Indices 

Natalia Zazulie, Francesca Raffaele, and Erika Coppola

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

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

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

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

EGU26-21830 | ECS | Posters virtual | VPS23

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

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

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

 

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

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

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

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

EGU26-23043 | Posters virtual | VPS23

Analysis of Vector-Field Multifractal Cascades 

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

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

NP1 – Mathematics of Planet Earth

EGU26-512 | ECS | Posters on site | NP1.1

Hybrid metaheuristic optimization for variational data assimilation in turbulence reanalysis 

Grzegorz Zakrzewski and Jacek Mańdziuk

The 3D-Var method for data assimilation estimates atmospheric states by minimizing a cost function that measures the mismatch between model forecasts and observations, weighted by their error covariances. Standard implementations employ preconditioned conjugate-gradient (CG) solvers. CG performs well for quadratic cost functions under Gaussian error assumptions, but in nonlinear or non-Gaussian settings, the overall minimization process may converge to suboptimal local minima. These conditions are characteristic of aviation turbulence assimilation, where measurements are spatially and temporally sparse, exhibit heterogeneous uncertainty, and involve nonlinear relationships between observed quantities and model states.

This study develops a turbulence reanalysis by assimilating Eddy Dissipation Rate forecasts from the COSMO time-lagged ensemble with turbulence observations derived from Mode-S EHS radar, as well as AMDAR and AIREP reports. To address the limitations of CG-based optimization in this nonlinear, non-Gaussian setting, we implement a hybrid metaheuristic framework combining Simulated Annealing, Particle Swarm Optimization, and Differential Evolution with local Quasi-Newton methods. The algorithm dynamically exchanges information between exploration and exploitation phases to avoid premature convergence to suboptimal solutions.

We benchmark the hybrid metaheuristic 3D-Var against the conventional CG approach, evaluating convergence characteristics, computational efficiency, and accuracy of analysis. Results will demonstrate whether the hybrid approach can improve solution stability and quality in nonlinear, non-Gaussian data assimilation problems.

How to cite: Zakrzewski, G. and Mańdziuk, J.: Hybrid metaheuristic optimization for variational data assimilation in turbulence reanalysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-512, https://doi.org/10.5194/egusphere-egu26-512, 2026.

EGU26-1540 | ECS | Posters on site | NP1.1

Quasipotential analysis of tipping points for a box model of the Atlantic Meridional Overturning Circulation 

Ruth Chapman, Peter Ashwin, and Richard Wood

A non-autonomous system can undergo a rapid change of state in response to a small or slow change in forcing, due to the presence of nonlinear processes that give rise to critical transitions or tipping points. Such transitions are thought to exist in various subsystems (tipping elements) of the Earth’s climate system. The Atlantic Meridional Overturning Circulation (AMOC) is considered a particular tipping element where models of varying complexity have shown the potential for bi-stability and tipping. Quasipotentials are a useful mathematical tool for understanding the ‘potential’ of such a system, where the potential cannot be calculated analytically, or may not exist. Quasipotentials can be used to calculate useful features such as minimum action paths and transition times, based on a purely stochastically forced system. In this work, we utilise an Ordered Line Integral Method (OLIM) of Cameron et.al. (2017) to estimate quasipotentials for a 2-dimensional AMOC box model with anisotropic noise estimated from complex model output. We also examine how the quasipotential depends on the anisotropy of the noise, calculate minimum action paths between stable states for these various scenarios, and how the quasipotential changes as an external forcing is increased. We also extend this model and the OLIM to 3-dimensions and explore different statistical features.

How to cite: Chapman, R., Ashwin, P., and Wood, R.: Quasipotential analysis of tipping points for a box model of the Atlantic Meridional Overturning Circulation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1540, https://doi.org/10.5194/egusphere-egu26-1540, 2026.

EGU26-1795 | Posters on site | NP1.1

Stochastic Energy-Balance Model With A Moving Ice Line 

Ilya Pavlyukevich

In SIAM J. Applied Dynamical Systems, 12 (2013), pp. 2068-2092, Widiasih proposed and analyzed a deterministic one-dimensional Budyko-Sellers energy-balance model with a moving ice line. In the present paper, we extend this model to a stochastic setting and study it within the framework of stochastic slow-fast systems. In the limit of a small parameter, we derive the effective ice-line dynamics as a solution to a stochastic differential equation. This stochastic formulation enables the investigation of coexisting (metastable) climate states, transition dynamics between them, stationary distributions, bifurcations, and the system’s sensitivity to perturbations. This talk is based on the joint work with M. Ritsch, SIAM J. Applied Dynamical Systems, 23(3), pp. 2061-2098.

How to cite: Pavlyukevich, I.: Stochastic Energy-Balance Model With A Moving Ice Line, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1795, https://doi.org/10.5194/egusphere-egu26-1795, 2026.

EGU26-2772 | ECS | Orals | NP1.1

Regime persistence through noise - A data-driven approach using deterministic trajectories 

Henry Schoeller, Robin Chemnitz, Péter Koltai, Maximilian Engel, and Stephan Pfahl

We investigate the lifetime of dynamical regimes under the impact of noise motivated by models of the atmosphere. One may expect that the inclusion of noise tends to make the system leave prescribed regions of the state space faster. However, for relevant systems with complexities ranging from phenomenological toy models to models of atmospheric dynamics, this intuition has proven misleading. As long as the noise is sufficiently small, the noisy system stays in regimes of interest on average longer than its deterministic counterpart, an effect we call "stochastic inertia''. This phenomenon has been observed through extensive numerical simulations for different noise levels. We propose a numerical technique for testing the occurrence of stochastic inertia, constructing, for any fixed noise level, a Markov chain on the set of points given by a  sufficiently long trajectory of the system without noise. The method is shown to correctly predict the presence of stochastic inertia in simple systems, and its utility is demonstrated on a paradigm model of atmospheric dynamics.

How to cite: Schoeller, H., Chemnitz, R., Koltai, P., Engel, M., and Pfahl, S.: Regime persistence through noise - A data-driven approach using deterministic trajectories, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2772, https://doi.org/10.5194/egusphere-egu26-2772, 2026.

EGU26-3556 | Orals | NP1.1

On the benefits of assimilating clear-sky radiances every 75 km globally at sub-hourly time scales 

Josef Schröttle, Cristina Lupu, and Chris Burrows

A refined 4D-Var assimilation system within DestinE allows us to assimilate the Meteosat-10/SEVIRI clear-sky radiances over Europe, as well as globally at a spatial scale of 75 km instead of the previous 125 km in the ECMWF Integrated Forecasting System (IFS). Higher resolution observations can potentially improve the analysis and therefore the prediction of extreme weather events over Europe, as well as globally. The effects of using higher resolution observations have been investigated with a detailed set of experiments and the impact on wind, temperature, and humidity has been evaluated. A broad range of experiments indicate that exploiting the higher spatial density clear-sky radiances leads to an improvement of humidity sensitive fields in short-range forecasts with the IFS as independently measured for example by instruments on low-Earth-orbiting satellites (IASI, CrIS, SSMIS, or ATMS). Due to a reduced representativeness error, these changes further lead to improvements in longer range forecasts as these errors would propagate upscale nonlinearly. Our experiments show an upscale propagation of initially very localised increments in the analysis fields of vertical wind, as well as humidity above the Pacific or the North Atlantic. Over the first 25 days of cycling, these incremental improvements from the 4D-Var system lead to an improvement in forecast scores of the IFS. Such a configuration with globally denser radiances will go into the next IFS Cycle 50r1. In the DestinE 4 km analysis, spatial error correlations are significantly reduced, e.g., for Meteosat-10/SEVIRI above Europe, highlighting the potential of high resolution data assimilation, as a reduction in spatially correlated errors leads to more accurate inital conditions, and globally improved forecasts up to 5 days ahead.

For the chosen configuration with spatially denser observations every 75 km globally at the sub- mesoscale, we focus on assimilating geostationary satellite observations at sub-hourly timescales every 10 minutes. For that purpose, we assimilate the pre-processed GOES-16-18/ABI observations by NOAA, as well as HIMAWARI-9/AHI by the Japanese Meteorological Agency (JMA), every 10 min, 20 min and 30 min. Exploring how to best assimilate relatively small spatial and temporal scales for these geostationary satellites, will allow us to approach a higher resolution for the whole MTG/FCI satellite series above Europe. Thereby, single cycle experiments with a 4 km global analysis reveal the impact of wind tracing in 4D-Var. In combination with the spatially and temporally denser observations, we further discuss the impact of diabatic heating on the role of establishing a meridional circulation that significantly improves wind, temperature and humidity over the southern oceans.

How to cite: Schröttle, J., Lupu, C., and Burrows, C.: On the benefits of assimilating clear-sky radiances every 75 km globally at sub-hourly time scales, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3556, https://doi.org/10.5194/egusphere-egu26-3556, 2026.

EGU26-4078 | ECS | Posters on site | NP1.1

Residual Ordering of Koopman Spectra for the Identification of Tropical Fundamental Modes 

Paula Lorenzo Sánchez, Matthew Colbrook, 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 approaches, have enabled exploration of nonlinear ENSO-related modes. However, they 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 DMD framework as a tool to classify and prioritize modes based on their residuals. Together with the application of pseudospectrum theory, 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 ResDMD, is capable of isolating fundamental modes of tropical SST dynamics. These modes not only provide insights into the system’s physical evolution but also prove highly effective in reproducing the Niño3.4 index and in generating forecasts that outperform state-of-the-art LIM-based predictions. By systematically identifying, interpreting, and exploiting these 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 ResDMD to refine mode selection in Koopman spectral analysis, paving the way for robust, physically interpretable, and predictively powerful insights into tropical SST variability.

How to cite: Lorenzo Sánchez, P., Colbrook, M., and Navarra, A.: Residual Ordering of Koopman Spectra for the Identification of Tropical Fundamental Modes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4078, https://doi.org/10.5194/egusphere-egu26-4078, 2026.

EGU26-4443 | ECS | Orals | NP1.1

Machine-Precision Prediction of Low-Dimensional Chaotic Systems 

Christof Schötz and Niklas Boers

Data-driven emulation of chaotic dynamics in the Earth system is a central challenge in modern climate science. Low-dimensional systems such as the Lorenz-63 model, derived in the context of atmospheric convection, are commonly used to benchmark system-agnostic methods for learning dynamics from data. Here we show that learning from noise-free observations in such systems can be achieved up to machine precision: using ordinary least squares regression on high-degree polynomial features with 512-bit arithmetic, our system-agnostic method matches the accuracy of standard numerical ODE solvers using the systems' governing equations. For the Lorenz-63 system, we obtain valid prediction times of 36 Lyapunov times, and even up to 105 Lyapunov times with favorable precision configurations, dramatically outperforming prior work, which reaches 13 Lyapunov times at most. We further validate our results on Thomas' Cyclically Symmetric Attractor, a non-polynomial chaotic system that is considerably more complex than the Lorenz-63 model, and show that similar results extend to higher dimensions using the spatiotemporally chaotic Lorenz-96 model. Our findings suggest that learning low-dimensional chaotic systems from noise-free data is a solved problem.

How to cite: Schötz, C. and Boers, N.: Machine-Precision Prediction of Low-Dimensional Chaotic Systems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4443, https://doi.org/10.5194/egusphere-egu26-4443, 2026.

EGU26-4975 | ECS | Posters on site | NP1.1

Analysis of Forecast Error Growth in Atmospheric Multiscale Lorenz Systems 

Hynek Bednar and Holger Kantz

In classical low‑dimensional chaotic systems, small initial‑condition errors grow exponentially on average in the tangent‑linear regime, with a rate set by the leading Lyapunov exponent, before entering a nonlinear regime in which the growth follows a quadratic law and saturates at a finite error amplitude. In systems with coupled temporal and spatial scales, the growth of initial‑condition errors is scale‑dependent and is most appropriately described by a power‑law behavior. We demonstrate how the parameters of the power law are linked to the intrinsic properties of individual scales and to the coupling between them. In systems where the model does not perfectly represent reality due to the omission of small temporal and spatial scales, the mean growth of model error (in the absence of initial‑condition error) can be approximated by a quadratic law with an additional parameter characterizing model error. To describe this process, we extend Orrell’s definition of drift by interpreting its generation at each time step, within our hypothesis, as an effective initial‑condition error that evolves according to classical chaotic growth. Based on this hypothesis, we explain the values of the parameters governing the model‑error growth law. The interpretations of the parameters and the underlying hypotheses are tested using multiscale atmospheric Lorenz systems. 

How to cite: Bednar, H. and Kantz, H.: Analysis of Forecast Error Growth in Atmospheric Multiscale Lorenz Systems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4975, https://doi.org/10.5194/egusphere-egu26-4975, 2026.

EGU26-5109 | Orals | NP1.1

Assessment of the predictability of cold-wet-windy Pan Atlantic compound extremes 

Meriem Krouma and Gabriele Messori

Occurrence of cold spells in different North American regions has been related to concurrent wet and windy extremes in Western Europe. This link is driven by an anomalous state of the North Atlantic storm track. Two dynamical pathways have been defined as potential origins of the Pan-Atlantic compound extremes. The first pathway is linked to a Rossby wave train propagating from the Pacific toward the Atlantic, associated with a pronounced Alaskan ridge. The second pathway is characterized by the presence of a high west of Greenland, that favors simultaneously a southward displacement of a trough over eastern USA and an upper level trough over South western Europe. This study investigates the predictability of flow associated with cold spells over north America from a dynamical systems perspective, with a focus on the underlying diversity of atmospheric states and wave processes.

We start by assessing the intrinsic predictability of these two pathways using the ERA5 reanalysis and dynamical systems indicators. These indicators can be used as proxies for the predictability of each pathway. We also examine the predictability of those two pathways across different climatological periods. We further explore how variations in Rossby wave behavior and stratospheric anomalies modulate the predictability of these cold spells. We complement this analysis using the ECMWF ensemble reforecasts at different lead times, and computing skill scores for the two pathways. This help to provide new insights into the dynamical precursors and sources of predictability for compound cold and windy extremes across the North Atlantic sector.

How to cite: Krouma, M. and Messori, G.: Assessment of the predictability of cold-wet-windy Pan Atlantic compound extremes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5109, https://doi.org/10.5194/egusphere-egu26-5109, 2026.

EGU26-5179 | ECS | Posters on site | NP1.1

A dynamical systems analysis of deep ocean convection with applications to the subpolar North Atlantic 

Scott Lewin, Marilena Oltmanns, Chris Wilson, Pavel Berloff, and Ted Shepherd

Ocean convection is an essential component of the climate system. In the Labrador Sea of the North Atlantic, convection can be particularly deep and intense, forming the downward branch of the Atlantic Meridional Overturning Circulation (AMOC). Increased freshwater input to the Labrador Sea resulting from melting Greenland ice caps puts convection at risk of shutting down. This could weaken the AMOC and would have wide impacts on global climate. Here, we represent ocean convection in a two-box model with seasonal forcing. The model may exhibit various convective regimes, including where convection is permanently shut down. Despite its simplicity, the model reproduces the observed variability well. We explore the possible climate regimes of the two-box model by fitting its parameters to a variety of observation-based datasets, including the Arctic Subpolar gyre sTate Estimate (ASTE), gridded Argo data and CMEMS reanalysis. We construct bifurcation diagrams showing the proximity of the system to a deep convective shutdown. Results suggest that in the Labrador Sea this shutdown is not as close as suggested in previous literature. Our approach allows a deeper understanding of the dynamics of a deep convective shutdown and provides improved estimates of deep convective stability.

How to cite: Lewin, S., Oltmanns, M., Wilson, C., Berloff, P., and Shepherd, T.: A dynamical systems analysis of deep ocean convection with applications to the subpolar North Atlantic, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5179, https://doi.org/10.5194/egusphere-egu26-5179, 2026.

EGU26-5296 | ECS | Orals | NP1.1

Changes in atmospheric circulation patterns are associated with increased European heat-related mortality 

Emma Holmberg, Joan Ballester, Davide Faranda, Raúl Méndez Turrubiates, and Gabriele Messori

Heat poses a critical risk to human health around the world. Recent work has investigated how anthropogenic climate change can modulate atmospheric circulation patterns, finding that circulation patterns increasing in frequency are associated with high temperatures in Europe. Here, we investigate the role of these changes in the dynamics of the atmosphere for European heat-related mortality. Specifically, we identify circulation patterns whose occurrence has become either more or less frequent over past decades. We couple this with an epidemiological framework, which uses an advanced regression model to compute associations between temperature and mortality. This association accounts for lags extending up to three weeks, and is fit for each subnational region within our dataset, which covers almost all of Europe. This allows us to estimate the heat-related mortality burden associated with circulation patterns that have changed in frequency. We find that dynamical changes have reinforced the thermodynamic warming trend, and are associated with increased heat-related mortality in northern and central continental Europe. Furthermore, dynamical changes appear to have played an important role for the extreme temperatures of the European summer of 2003, and the associated heat-related mortality. We thus highlight the importance of considering the role of changes in atmospheric circulation patterns when investigating the role of climate change for heat events and their impacts. Furthermore, we argue that heat action plans should consider the possibility of record-shattering heat events, where dynamical changes contributing to anomalously high temperatures could coincide with the peak of the seasonal temperature cycle, as seen in 2003. 

How to cite: Holmberg, E., Ballester, J., Faranda, D., Méndez Turrubiates, R., and Messori, G.: Changes in atmospheric circulation patterns are associated with increased European heat-related mortality, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5296, https://doi.org/10.5194/egusphere-egu26-5296, 2026.

This study introduces a new methodology for diagnosing atmospheric circulation associated with surface extremes in modal space. The approach is conceptually similar to spherical harmonics analysis but employs Hough harmonics as basis functions. These harmonics arise from the linearised primitive equations and form an orthogonal basis. Projection onto this basis yields complex Hough expansion coefficients that describe the amplitudes and phases of the modal contributions to the global three-dimensional fields. Each Hough coefficient is indexed by zonal wavenumber, meridional mode, and vertical structure function. The orthogonality of the modes allows a decomposition of the total energy into the energy of the zonal mean flow and the energies of different wave components.

The method is applied to global reanalysis datasets and to a subset of CMIP5 climate model simulations from 1980 onwards. Reconstructed circulation fields, obtained by inverse projection onto wind and geopotential using scale-selective filtering, indicate that Eurasian heatwaves (EHWs) are primarily driven by large-scale anticyclonic systems. This agrees with previous dynamical studies and supports the physical interpretability of the diagnostic. Probability distribution functions of Rossby wave energies are computed separately for the zonal mean, for planetary-scale, and for synoptic-scale zonal wavenumbers, focusing on barotropic structures in the troposphere. The corresponding energy time series are well described by chi-square distributions, and the skewness indicates about a 50% reduction in the effective degrees of freedom of planetary-scale circulation during EHWs.

This reduction is not observed in the CMIP5 simulations, which points to systematic model deficiencies. The models reproduce present-day surface EHW characteristics and associated Rossby wave patterns reasonably well, but struggle to reproduce day-to-day circulation variability observed in reanalyses. This limitation reduces confidence in projections of future changes in heatwaves and their related large-scale circulation. The results suggest that metrics describing intrinsic variability should be included as complementary to existing ones when evaluating simulations of heatwaves and associated circulation.

Overall, the diagnostic provides a holistic dynamical view of the variability spectrum of Rossby waves linked to surface extremes. It enables scale-selective filtering of variability in physical space and reveals statistical properties in modal space, offering a useful tool for model assessment and for studying complex atmospheric dynamics.

How to cite: Strigunova, I.: Modal-space statistics of Rossby waves during Eurasian heatwaves: implications for circulation dynamics in reanalyses and climate models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5650, https://doi.org/10.5194/egusphere-egu26-5650, 2026.

Connecting the different levels of the hierarchy of mathematical and conceptual complexity at which climate models operate, and comparing the assumptions that apply at each level, and the results produced, 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) and its successors . Another informative, but lateral, connection and comparison is that between either studying climate through the lens of stochastic physical models and 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 ARIMA model with automatically selected parameters I will show that in this instance the absence of a prominent autoregressive term can have quite the opposite meaning and  instead be a clear indication of strong driving. I will present results of our ensemble study which is examining the ability of automatic fitting to correctly infer ARIMA parameters on EBMs with realistic values of heat capacity and other system variables. Progress in extending the study to fractional EBMs and to ARFIMA models will be discussed.

 

How to cite: Watkins, N. W. and Stainforth, D.: What do we learn from looking at the Hasselmann model through 2 lenses ? Stochastics meets statistics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5791, https://doi.org/10.5194/egusphere-egu26-5791, 2026.

Sea ice is a multiscale composite displaying complex structure on length scales ranging over many orders of magnitude. Finding the effective properties relevant to large-scale dynamics and thermodynamics is a central challenge in modeling and predicting sea ice behavior, similar to finding macroscopic behavior from microscopic laws in statistical mechanics. Integral representations for the homogenized properties of composites, where the microstructural geometry is encoded into the spectrum of a random operator, have opened up new theoretical and computational approaches to sea ice modeling. We’ll give an overview of how they’re being used to study sea ice electromagnetics, thermal transport, wave-ice interactions, and advection diffusion processes at the floe scale. They also allow us to connect sea ice to random matrix theory, uncertainty quantification, and exotic materials such as twisted bilayer graphene.

How to cite: Golden, K.: Multiscale homogenization and random matrix theory for sea ice, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6058, https://doi.org/10.5194/egusphere-egu26-6058, 2026.

This study introduces a novel sequential data assimilation method that uses conditional denoising score matching (CDSM). The CDSM leverages iterative refinement of noisy samples guided by conditional score functions to achieve real-time state estimation by incorporating observational constraints at each time step. Unlike traditional methods, such as variational assimilation and Kalman ffltering, which rely on Gaussian assumptions and can be computationally expensive because of iterations or ensembles, CDSM is based on stochastic differential equations (SDEs). It does not require explicit noise addition or manipulation of probability density functions, thus simplifying the assimilation process and enhancing the computational efficiency. Here, error growth and reduction were modeled using noise addition and denoising processes based on SDEs. This transforms the data assimilation problem into a denoising problem based on conditional score matching. Our approach integrates dynamic models, performs data assimilation through Langevin dynamics at the observation times, and uses the analyzed states for subsequent integration. The noise addition process is embedded in the score model training using neural networks and is not explicitly used in the assimilation process. The results from twin experiments using the Lorenz ‘63 model demonstrate that the CDSM achieves a performance comparable to that of traditional methods in nonlinear systems. This method is robust and flexible with low requirements for training data quality. This is particularly suitable for scenarios in which the observation intervals are much larger than the model integration steps. The CDSM shows great potential for application inlarge-scale numerical and data-driven models.

How to cite: Shen, Z.: A Novel Sequential Data Assimilation by Conditional Denoising Score Matching, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6704, https://doi.org/10.5194/egusphere-egu26-6704, 2026.

Coarse-grained models of chaotic systems neglect unresolved degrees of freedom, inducing structured model error that limits predictability and distorts long-term statistics. Standard data-driven closures address this by training offline to minimize one-step prediction error, implicitly assuming Markovian dynamics and deterministic corrections. Here we demonstrate that this paradigm is fundamentally flawed. Using mesoscale turbulence as a canonical multiscale system, we show that offline training yields poorly calibrated forecasts and incorrect stationary statistics, regardless of model complexity. In contrast, stochastic closures trained on trajectories using proper scoring rules recover reliable ensemble forecasts and realistic long-term behavior. We find that this improvement stems not from architectural sophistication, but from probabilistic calibration over multiple time steps. Our results identify online (trajectory-based) learning and stochasticity as structural requirements for representing unresolved dynamics, with significant implications for Earth system modelling and data-driven prediction more broadly.

How to cite: Brolly, M.: Trajectory-based probabilistic learning is essential for representing unresolved dynamics in chaotic systems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6847, https://doi.org/10.5194/egusphere-egu26-6847, 2026.

EGU26-7147 | Posters on site | NP1.1

Stable gradient-wind balance at high Rossby numbers: A semi-implicit method applied to high-resolution Ocean satellite data 

Jeremy Collin, Anastasia Volorio-Galéa, and Pascal Rivière

The 2022 launch of the SWOT satellite (Surface Water and Ocean Topography) enabled sea surface height observations at unprecedented high resolution of approximately 2 km. These measurements are used to generate sea surface current maps by applying the geostrophic balance equation. At these fine scales, intense small-scale eddies become visible. These eddies exhibit strong ageostrophic behavior driven by non-linear advection, with Rossby numbers larger than 1. Theoretical work indicates that geostrophic current estimates can overestimate or underestimate actual current velocities by approximately a factor of 2 for ageostrophic cyclones and anticyclones respectively. This makes solving the gradient-wind equation essential for accurate representation. Earlier efforts to address this challenge employed explicit iterative finite difference schemes, which are known to lose stability when Rossby numbers exceed 1. We present a novel approach using a semi-implicit finite difference method. Our method is first tested against analytical solutions in a simplified framework, then validated using a 1 km resolution primitive equation ocean model. We demonstrate the method's application to SWOT observations of an intense oceanic submesoscale cyclone.

How to cite: Collin, J., Volorio-Galéa, A., and Rivière, P.: Stable gradient-wind balance at high Rossby numbers: A semi-implicit method applied to high-resolution Ocean satellite data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7147, https://doi.org/10.5194/egusphere-egu26-7147, 2026.

EGU26-7720 | ECS | Orals | NP1.1

Accelerated Bayesian Optimisation for bias correction in an Intermediate Complexity Climate Model 

Valérian Jacques-Dumas, Henk A. Dijkstra, and Jeanne Vedel

One of the main issues faced by climate models is the presence of biases due to uncertainties in model parameters. Here, we set out to constrain such parameter values by reducing the mismatch between a climate model's equilibrium state and ground-truth observations through the minimisation of a cost function, using Bayesian optimisation. We illustrate this method on the parametrisation of the ocean vertical diffusivity $\kappa$, first as a proof-of-concept in a conceptual ocean model, then in VEROS, a global ocean model of intermediate complexity. In the first case, we can artificially introduce an error in $\kappa$ and show that Bayesian optimisation allows us to retrieve its true value. In the case of VEROS, we aim at improving the model's description of the Atlantic Meridional Overturning Circulation (AMOC), so we can compare the simulated AMOC strength to the measured mean AMOC strength over the past two decades.

However, the equilibrium state of a model depends on the model parameters. Since we are modifying these parameters at each Bayesian iteration, the equilibrium state of the model needs to be recomputed every time in order to be compared to observations. In climate models, equilibria are usually computed through spin-ups, or trajectories of typically several thousands of years. But this method is extremely costly and does not guarantee that all model variables have converged to the equilibrium, since they evolve on a large range of time scales. On the other hand, Anderson Acceleration (AA) is an iterative method designed to solve fixed-point equations for any dynamical system much more efficiently than using direct integration. Indeed, AA determines at each iteration an educated guess of the position of the equilibrium by combining previous iterates. Here, we combine AA and Bayesian optimisation to re-compute the model's equilibrium at every Bayesian iteration. We show that we are able to constrain the distribution of $\kappa$ values to minimise the distance to observations.

But this process still requires running the model a large number of times at each Bayesian iteration, which remains computationally costly. To reduce the computational burden even further, we train a deep machine learning (ML) scheme to reconstruct the entire state vector of the model from a few significant fields, such as temperature and salinity, that most contribute to the large-scale dynamics of the system. This ML scheme therefore acts as an emulator of the climate model, which does not need to perfectly reproduce all processes, but mostly the model's equilibria. AA is then applied to these few fields only, while the full model state is reconstructed by the ML scheme at each AA iteration.

How to cite: Jacques-Dumas, V., Dijkstra, H. A., and Vedel, J.: Accelerated Bayesian Optimisation for bias correction in an Intermediate Complexity Climate Model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7720, https://doi.org/10.5194/egusphere-egu26-7720, 2026.

EGU26-9418 | ECS | Posters on site | NP1.1

Barotropic-Baroclinic Splitting for Multilayer Shallow Water Models with Exchanges 

Sophie Hörnschemeyer, Nina Aguillon, and Jacques Sainte-Marie

Multilayer ocean models (see e.g. Audusse et al., ESAIM: Mathematical Modelling and Numerical Analysis 2011) are popular approximations to the 3D Euler and Navier-Stokes equations. Computational cost obviously increases with the number of layers, which is often chosen to be around 50 in ocean simulations. The barotropic-baroclinic splitting is an important strategy used in numerical ocean models to reduce this computational cost (see e.g. Killworth et al., Journal of Physical Oceanography 1991).

In the present contribution, we focus on the numerical analysis of the barotropic-baroclinic splitting in the context of finite volume schemes. We reformulate the splitting strategy within the nonlinear multilayer framework using terrain-following coordinates, and present it as an exact operator splitting. The barotropic step captures the evolution of free surface and depth averaged velocity with a well-balanced one-layer shallow water model. The baroclinic step incorporates vertical exchanges between layers and adjusts velocities around their mean vertical value.

Our scheme is numerically robust, i.e. no filters or corrections are needed. The numerical solution inherently observes a discrete maximum principle for the tracer and hence guarantees non-negative tracer concentrations. In the language of applied mathematics, we prove a discrete entropy inequality. In the language of geophysics, this guarantees dissipation of kinetic and potential, and therefore of total energy. This is the key stability property for the class of finite volume schemes under consideration. Last, but not least, the gain in terms of computational cost is large, especially in low Froude simulations.

Currently, this work addresses the constant density case; however, ongoing work extends the barotropic-baroclinic splitting to variable density scenarios and models situations such as coastal upwelling. The paper is submitted for publication (Aguillon, Hörnschemeyer, Sainte-Marie, International Journal for Numerical Methods in Fluids, January 2026).

How to cite: Hörnschemeyer, S., Aguillon, N., and Sainte-Marie, J.: Barotropic-Baroclinic Splitting for Multilayer Shallow Water Models with Exchanges, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9418, https://doi.org/10.5194/egusphere-egu26-9418, 2026.

EGU26-9626 | Orals | NP1.1

Can we define climate by means of an ensemble? A tale of time scales of convergence 

Gábor Drótos and Tamás Bódai

It is hardly questioned today that climate can be described in theory by an ensemble of trajectories differing in their initial conditions, which is then translated to numerical ensembles in climate models. It is also widely accepted that any evolution observed within a few decades after initialization is not relevant to climate. Evolution at a later stage, instead, is then used to characterize climate and its change, under the implicit assumption that slower processes do not considerably contribute to differences between ensemble members, letting internal variability of climate be identified with these differences. However, a justification for this practice is as yet lacking. In particular, a definition of climate in support of this practice is outstanding, including the identification of the kind of time scales at play through providing an argumentation for their relevance. Our study aims at filling this gap. After pointing out that the most important criterion for a definition of climate is the uniqueness of the probability measure on which the definition relies, we first recall the naive proposal to represent such a probability measure by the distribution of ensemble members that has, loosely speaking, converged to the natural probability measure of the so-called snapshot or pullback attractor of the dynamics. We then consider the time scales of convergence and refine the proposal by taking a probability measure that is conditional on the (possibly time-evolving) state of modes characterized by convergence time scales longer than the horizon of a particular study. We design an ensemble simulation initialization scheme for studying convergence time scales and uniqueness of ensembles in Earth system models.

How to cite: Drótos, G. and Bódai, T.: Can we define climate by means of an ensemble? A tale of time scales of convergence, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9626, https://doi.org/10.5194/egusphere-egu26-9626, 2026.

EGU26-10391 | Orals | NP1.1

Nonlinear wave interactions in Rotating Shallow Water Equations on the Sphere: Theory and multi-wave applications 

Pedro Peixoto, Marco Dourado, Breno Raphaldini, and André Teruya

One of the challenges in weather forecasting is the understanding of the nonlinear interactions between the fast and slow dynamics in the atmosphere. This is related to both numerical problems, such as the choice of a stable time step, and modelling and understanding the dynamics of atmospheric phenomena, such as the Madden-Julian Oscillation. Using a Rotating Shallow Water model on the sphere, in which both fast (inertia-gravity) and slow (Rossby-Haurwitz) waves occur, the nonlinear interactions in reduced models containing three, four and five waves were analysed using Hough harmonics spectral decomposition. Considering a Galerkin expansion as a solution of the nonlinear system, equations for the dynamics of each mode were derived, along with necessary conditions in the zonal and meridional structure of the modes for three interacting waves. In this talk, we will show results of three, four and five wave system interaction, discussing the energy transfers between Rossby-Haurwitz and gravity waves. We will particularly illustrate how we can observe relevant slow oscillations emerging from fast wave dynamics in realistic parameter ranges.

How to cite: Peixoto, P., Dourado, M., Raphaldini, B., and Teruya, A.: Nonlinear wave interactions in Rotating Shallow Water Equations on the Sphere: Theory and multi-wave applications, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10391, https://doi.org/10.5194/egusphere-egu26-10391, 2026.

EGU26-10479 | Posters on site | NP1.1

Local kinetic energy fluxes in the atmospheric mesoscales 

Hannah Christensen, Salah Kouhen, Benjamin Storer, Hussein Aluie, and David Marshall

The mesoscale atmospheric energy spectrum has puzzled scientists for decades, sitting between classical turbulence and wave theories. Using year-long ECMWF operational analyses of high resolution and a spherical coarse-graining framework (Flowsieve), we present the first consistent global maps of local mesoscale kinetic energy fluxes. At 200~hPa, we identify a striking band of upscale transfer aligned with the ITCZ, while storm tracks and orography leave distinct dynamical imprints at both 200 and 600~hPa. By decomposing divergent and rotational components, we show that divergent energy dominates in the tropics and stratosphere, while rotational energy dominates in the extratropical troposphere. Conditioning spectra on this balance reveals contrasting regimes: a Nastrom–Gage-like spectrum under divergent dominance, and a spectrum reminiscent of the classical dual cascade of textbook two-dimensional turbulence under rotational dominance at 600~hPa. These results demonstrate that mesoscale energy transfer is shaped by a patchwork of mechanisms, reconciling long-standing debates and providing new inspiration for parametrisations and predictability in weather and climate models.

How to cite: Christensen, H., Kouhen, S., Storer, B., Aluie, H., and Marshall, D.: Local kinetic energy fluxes in the atmospheric mesoscales, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10479, https://doi.org/10.5194/egusphere-egu26-10479, 2026.

EGU26-10906 | ECS | Posters on site | NP1.1

A Diagnostic Framework for Spectral Biases in Fast Radiative Transfer Models: An ANOVA-based Uncertainty Decomposition of RTTOV 

Viviana Volonnino, Jean-Marie Lalande, and Jérôme Vidot

RTTOV is the operational fast radiative transfer model used as the forward operator in data assimilation systems at major NWP centres, including Météo-France and ECMWF. Its accuracy plays a crucial role in the evaluation and representation of observation errors. For instance, any limitations of its transmittance model can introduce systematic biases in the simulated brightness temperatures. These biases may propagate through the assimilation system, affecting both the retrieved atmospheric fields and the performance of the bias correction scheme.

Estimating and attributing biases in fast RT simulations remains challenging due to the complex and interacting error sources. In this study, we present a new ANOVA-style methodology to diagnose and separate these sources of biases using reference line-by-line models, satellite observations, and 1D-Var retrievals. We focus on three main contributors: spectroscopy, transmittance parametrisation, and uncertainties in atmospheric profiles. By analysing spectral biases across channels, gas absorption bands, and atmospheric regimes (e.g., dry, humid, tropical, polar), we identify dominant error sources and their impact on temperature and humidity retrievals.

Recent improvements in RTTOV coefficients and spectroscopy are also evaluated, demonstrating their impact on forward simulations for IASI (and prospectively FORUM) and on retrieved profiles. By isolating key error sources, this work strengthens the link between fast forward model development, bias correction schemes and retrieval accuracy.

How to cite: Volonnino, V., Lalande, J.-M., and Vidot, J.: A Diagnostic Framework for Spectral Biases in Fast Radiative Transfer Models: An ANOVA-based Uncertainty Decomposition of RTTOV, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10906, https://doi.org/10.5194/egusphere-egu26-10906, 2026.

EGU26-11347 | ECS | Posters on site | NP1.1

Nonlinear Atmospheric Inversion with Interpretable Bias Correction via Gaussian Process Prior 

Antonie Brožová, Václav Šmídl, Ondřej Tichý, and Nikolaos Evangeliou
Accurate quantification of atmospheric pollutant emissions is essential for evaluating the consequences of environmental incidents. Inverse modelling of such releases commonly employs a linear framework based on a source–receptor sensitivity (SRS) matrix; however, this matrix can be substantially biased or may even fail to represent the true scale of the release. We introduce a method in which the SRS matrix is corrected jointly with the inversion, resulting in a nonlinear inverse problem. The SRS discrepancies are interpreted as small shifts of observation points, leading to a deformation of the sensitivity field. The shifts are regularized through a Gaussian process prior, which imposes smoothness and sparsity while allowing inference at unobserved locations. The resulting posterior predictions of the shift field offer a practical tool for hyperparameter selection: the inferred shifts can be visualized geographically and evaluated by domain experts. This leads to a Bayesian framework that integrates inversion, SRS correction, and a tuning strategy based on L-curve-type diagnostics combined with maps of the predicted shifts. It will be demonstrated on a selected real continental-scale scenario of an atmospheric release.
 
This research has been supported by the Czech Science Foundation (grant no. GA24-10400S). FLEXPART model simulations are cross-atmospheric research infrastructure services provided by ATMO-ACCESS (EU grant agreement No 101008004). Nikolaos Evangeliou was funded by the same EU grant. The computations were performed on resources provided by Sigma2 - the National Infrastructure for High Performance Computing and Data Storage in Norway.

How to cite: Brožová, A., Šmídl, V., Tichý, O., and Evangeliou, N.: Nonlinear Atmospheric Inversion with Interpretable Bias Correction via Gaussian Process Prior, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11347, https://doi.org/10.5194/egusphere-egu26-11347, 2026.

EGU26-11361 | ECS | Orals | NP1.1

Dimension reduction Kalman filtering: examples from high-dimensional dynamical systems 

Tuukka Himanka and Marko Laine

We consider a prior-based dimension reduction Kalman filter for state estimation in high-dimensional settings. The method extend ideas from prior-based dimension reduction in static inverse problems by projecting covariance equations to lower-dimensional space using a global reduction operator. In contrast to reduced rank Kalman filters the dimension reduction is defined entirery a priori. Here, it is constructed using standard wavelet transforms, yielding a stable and portable framework that does not depend on empirical parameter estimation to form the projection. 

The Kalman filter update step equations are projected onto a global wavelet basis, thereby avoiding explicit construction of covariance matrices in the full state space. This makes classical Kalman filtering tractable for large spatio-temporal systems otherwise computationally inaccessible. Combined with PyTorch implementation exploiting GPU acceleration, the approach leads to a drastic reduction in computational cost, while preserving the consistent filter and enabling Gaussian uncertainty quantification.

We demonstrate the method on two high-dimensional application, highlightning the wavelet representation's natural adaptation to different data patterns and structures. The first example concerns sparsely observed oceanographic data, where the reduced filter reconstructs the full state from limited measurements with uncertainty estimates with state model derived from modelled ocean current. The second focuses on satellite-derived cloud product with state dynamics provided by neural network estimates and the observations exhibit heterrogeneous quality and frequent gaps.

Overall, we demonstrate how reduced-basis Kalman filtering with a priori selected wavelet subspaces provides a general and computationally viable framework for nonstationary Gaussian inverse problems. The approach combines scalable data assimilation, uncertainty quantification, and the integration of data-driven dynamics in high-dimensional geophysical applications.

How to cite: Himanka, T. and Laine, M.: Dimension reduction Kalman filtering: examples from high-dimensional dynamical systems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11361, https://doi.org/10.5194/egusphere-egu26-11361, 2026.

EGU26-11431 | ECS | Posters on site | NP1.1

A path-integral approach to coupled discrete-continuous problems 

Tobias Sparmann, Alexandra-Anamaria Sorinca, Michael te Vrugt, Gunnar Pruessner, Rosalba Garcia Millan, and Peter Spichtinger

Typical cloud physics systems at small scales are often formulated as coupled discrete–continuous problems, comprising discrete, stochastically evolving hydrometeors and continuous, field-like thermodynamic variables. For modeling purposes, the inherent stochastic and particle-based nature of these systems is frequently simplified into more tractable mathematical frameworks, such as moment-based schemes. However, such approximations often fail to adequately capture the full impact of stochastic effects and the structure of distribution tails – features that can significantly influence system behavior. Although these effects can be resolved at small scales through numerical simulations of Master equations and related methods, approaches to upscale such descriptions to large-scale systems have remained elusive.
In this work, we introduce a novel mathematical framework that translates general coupled discrete–continuous problems into a path integral formulation, and consequently into an approximate field theory. This approach circumvents the need for computationally expensive numerical simulations and enables direct analytical computation of distribution moments. As a result, parameter spaces of models can be efficiently explored via analytical means, facilitating their application to significantly larger spatial and temporal scales.
We illustrate the efficacy of our method using a simple model system and explore its applicability to typical atmospheric situations.

How to cite: Sparmann, T., Sorinca, A.-A., te Vrugt, M., Pruessner, G., Garcia Millan, R., and Spichtinger, P.: A path-integral approach to coupled discrete-continuous problems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11431, https://doi.org/10.5194/egusphere-egu26-11431, 2026.

EGU26-11895 | ECS | Orals | NP1.1

Dynamic Mode Decomposition with Control for Forced Response Estimation 

Nathan Mankovich, Andrei Gavrilov, and Gustau Camps-Valls

The problem of forced response estimation from a single realization was addressed in the recent ForceSMIP project [Wills et al. 2025], which compiles many state-of-the-art statistical methods, including both methods supervised by large Earth System Model (ESM) ensembles and methods that use only a single target climate realization. Single-realization estimation is frequently approached using various linear filtering techniques, in particular Linear Inverse Models (LIMs) and Dynamic Mode Decomposition (DMD) [Penland et al. 1995 and Schmid 2010]. Standard LIM and DMD do not explicitly account for external forcing. DMD with control (DMDc) naturally extends these methods to incorporate essential external forcing information as a control variable [Proctor et al. 2016].

We investigate how these forcing inputs can be incorporated into the DMDc model to estimate forced responses. This results in three variants of DMDc for forced response estimation. One variant was already used in Tier 1 of the ForceSMIP project, while the other two have yet to be tested. We evaluate all three methods using near-surface air temperature (tas) and sea-level pressure (psl) from four Earth system models (CanESM5, MIROC6, MPI-ESM, and MPI-ESM1-2-LR) using data from MMLEA v2 [Maher et al. 2025]. Specifically, we analyze their ability to recover forced responses and characterize the DMDc variants across these Earth system models and variables.

References:

    Maher, Nicola, et al. "The Updated Multi-Model Large Ensemble Archive and the Climate Variability Diagnostics Package: New Tools for the Study of Climate Variability and Change." Geoscientific Model Development 18.18 (2025): 6341-6365.

    Penland, Cécile, and Prashant D. Sardeshmukh. "The Optimal Growth of Tropical Sea Surface Temperature Anomalies." Journal of Climate 8.8 (1995): 1999-2024.

    Proctor, Joshua L., Steven L. Brunton, and J. Nathan Kutz. "Dynamic Mode Decomposition with Control." SIAM Journal on Applied Dynamical Systems 15.1 (2016): 142-161.

    Schmid, Peter J. "Dynamic Mode Decomposition of Numerical and Experimental Data." Journal of Fluid Mechanics 656 (2010): 5-28.

    Wills, Robert CJ, et al. "Forced Component Estimation Statistical Method Intercomparison Project (ForceSMIP)." Authorea Preprints (2025).

How to cite: Mankovich, N., Gavrilov, A., and Camps-Valls, G.: Dynamic Mode Decomposition with Control for Forced Response Estimation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11895, https://doi.org/10.5194/egusphere-egu26-11895, 2026.

The Atlantic meridional overturning circulation, the Greenland and Antarctic ice sheets have been identified as parts of the climate system that can potentially react nonlinearly to climate change albeit on very different time scales. While critical thresholds remain difficult to quantify from existing observations for all of these subsystems, they certainly do not stand on their own. In fact, the AMOC and polar ice sheets form an intricate network of multiscale systems, with interactions that can be stabilizing or destabilizing, the latter opening the possibility of cascading tipping events.

The interaction between Greenland ice sheet and AMOC on the larger scale shows the possibility of a collapse of the AMOC once a critical amount or rate of freshwater has entered the North Atlantic. This interaction also involves smaller scales, because the Greenland meltwater needs to reach the deep-water formation regions in the North Atlantic subpolar gyre, exhibiting substantial variability in the critical regions. Moreover, the Greenland ice sheet acts on slower time scales than the AMOC, such that these two systems can form an ‘accelerating cascade’. Specfically, when tipping of the ice is underway, the ‘coupling’, i.e. the freshwater flux into the North Atlantic is at maximum. These properties have consequences for the possibility of early warning predictions; in accelerating cascades early warning signs can break down due to lack of extrapolation.

On the other hand, West Antarctic Ice Sheet melting may be able to to stabilize the AMOC. Here, we investigate through a hierarchy of models of the AMOC and idealized forms of polar ice sheet collapse, the origin and relevance of stabilization and destabilization effects. In both deterministic and stochastic conceptual models, we find that rate- and noise-induced effects have substantial impact on the AMOC stability. Moreover, rate-induced effects can stabilize the AMOC depending on the relative timing of the peak meltwalter fluxes from both ice sheets.

How to cite: von der Heydt, A.: How stable is the Atlantic meridional ocean circulation when interacting with polar ice sheets?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12246, https://doi.org/10.5194/egusphere-egu26-12246, 2026.

EGU26-12391 | ECS | Posters on site | NP1.1

Towards inverse estimation of Spanish NOx emissions with TROPOMI observations using a variational autoencoder 

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

Air pollution estimates represent key inputs in computer models for assessing air quality. They are also important in the evaluation of pollution control policies. 

In the last decade, neural networks have demonstrated exceptional ability to model complex spatiotemporal data. Meanwhile, advances in our ability to observe the earth's atmosphere using satellites have enabled the collection of high-resolution atmospheric composition data in near real-time. These developments open up opportunities to combine the predictive power of neural networks with satellite observations to deliver rapid and accurate estimates of pollutant emissions in near real-time.

Chemical weather prediction models offer insights into the forward relationship between emissions and atmospheric composition, and some studies are already suggesting that neural networks 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 not. Our objective is ultimately to exploit neural networks to predict emissions from atmospheric composition. This presents challenges, as we will show in our presentation.

We present preliminary results from our study in training a variational autoencoder, with data from a chemical weather prediction model, to invert Spanish NOx emissions. We demonstrate a workflow in which we jointly train two neural network models: one for inverse modelling of emissions and a second to regularise the predictions of the inverse model.  

How to cite: Petticrew, J., Petetin, H., Mas Magre, I., Guevara Vilardell, M., Jorba, O., and Pérez García-Pando, C.: Towards inverse estimation of Spanish NOx emissions with TROPOMI observations using a variational autoencoder, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12391, https://doi.org/10.5194/egusphere-egu26-12391, 2026.

EGU26-12966 | ECS | Orals | NP1.1

Extending Cross Entropy Based Importance Sampling for Bayesian Updating (CEBU) with Empirical Priors and Kolmogorov-Smirnov Based Convergence Diagnostics 

Michael Engel, Sindhu Ramanath, Lukas Krieger, Jan Wuite, Dana Floricioiu, and Marco Körner

Bayesian inverse problems in Earth sciences often ask for inversion techniques capable of handling high-dimensional nonlinear forward models, and prior information that is neither Gaussian nor analytically representable. This contribution focuses on the methodological developments underlying our application of cross entropy based importance sampling for Bayesian updating (CEBU) to Antarctic tidal grounding line migration based upon Sentinel-1 line of sight offsets. In particular, we highlight how the algorithm is extended to incorporate empirical, hence, nonparametric priors, how its sequential structure enables detailed convergence diagnostics, and how its evidence estimate can support filtering and model selection.

The grounding line marks the transition from grounded ice to floating ice shelf in Antarctica’s marine-terminating glaciers. The underlying elastic beam model simulating the bending of the ice in response to tidal deflection is, among others, based on an ice thickness parameter. Its prior shall be defined by the values from a dataset of a previous study. This prior exhibits non‑Gaussian structure and parameter dependencies that cannot be captured by standard parametric assumptions. Hence, we extend the CEBU framework by introducing an isoprobabilistic transform that maps the empirical ensemble into the standard normal space in which the update is performed. The extension allows CEBU to operate directly on empirical prior information, thereby embedding physical knowledge into the Bayesian update in a fully nonparametric manner.

After the initial transformation to standard normal space, CEBU proceeds through a sequence of tempered intermediate distributions that gradually introduce the likelihood. This sequential structure provides a transparent view of convergence behavior: we introduce the Kolmogorov–Smirnov distance between each intermediate importance sampling density and the prior as a measure of information gain and respective parameter importance. This quantity provides a nonparametric and interpretable metric of which components of the parameter vector are most informed by our observations and which remain dominated by prior uncertainty. The difference of information gained per step determines the respective importance of a parameter at a particular tempering step. Hence, by the distance metric introduced, CEBU intrinsically provides a convergence curriculum used to attain the posterior distribution.

After convergence, CEBU yields a Bayesian model evidence estimate. It quantifies the conceptual fit of the data observed and the model used. Accordingly, this evidence can be used for filtering the results, e.g., if the observation data of a particular inverse problem is too noisy, i.e., does not follow the measurement error model. Further, that quantity may be used for Bayesian model selection, offering a principled mechanism for evaluating competing forward models or prior assumptions. For example, that setting can be used to decide between multiple empirical priors, and thus between competing studies.

From a computational perspective, all forward evaluations and likelihood computations are embarrassingly parallelizable. That makes the approach well suited for large‑scale inference tasks on modern high performance clusters and cloud infrastructures.

How to cite: Engel, M., Ramanath, S., Krieger, L., Wuite, J., Floricioiu, D., and Körner, M.: Extending Cross Entropy Based Importance Sampling for Bayesian Updating (CEBU) with Empirical Priors and Kolmogorov-Smirnov Based Convergence Diagnostics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12966, https://doi.org/10.5194/egusphere-egu26-12966, 2026.

EGU26-13629 | ECS | Orals | NP1.1

Extracting persistent topological modes of variability in complex dynamics from data 

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

Complex systems such as the climate are often described in terms of linear modes of variability, but these modes cannot capture the intrinsically nonlinear organization of the dynamics. We introduce a framework for extracting topological modes of variability (TMVs) directly from observational, laboratory or simulation data. 

TMVs were introduced in the context of the templex framework [Charó et al., 2022; 2025], which represents a dynamical system through a combination of its topological structure and the way the flow in phase space moves across it. In this framework, TMVs correspond to flow patterns that are organized around special regions of an attractor, called joining loci, where different pathways merge.

Here we show how these joining loci — and the TMVs organized around them — can be recovered directly from data, without explicitly constructing a cell complex. We use dynamical indicators of local dimension and stability [Lucarini et al., 2016; Faranda et al., 2017] to locate the regions of the attractor where joining loci are expected, and we then extract the corresponding cycles from a directed graph built on a clustering of the data. By retaining only the robust transitions in this graph, we obtain a set of persistent TMVs.

We apply this approach to the El Niño–Southern Oscillation (ENSO) using Niño-3.4 sea-surface temperature anomalies from NOAA’s Oceanic Niño Index (ONI), providing new insight into ENSO variability and predictability.

 

How to cite: Charó, G. D., Faranda, D., Ghil, M., and Sciamarella, D.: Extracting persistent topological modes of variability in complex dynamics from data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13629, https://doi.org/10.5194/egusphere-egu26-13629, 2026.

EGU26-13703 | Orals | NP1.1

Sea ice motion on multiple scales 

Srikanth Toppaladoddi

Arctic sea ice is one of the most sensitive components of the Earth's climate system and acts as a bellwether for changes in it. The ice cover grows, shrinks, and moves because of its interactions with the atmosphere and the underlying ocean. One of the principal challenges associated with modelling the atmosphere-ice-ocean interactions is the lack of definitive knowledge of the rheological properties of the ice cover at large scales. A systematic study of sea ice dynamics since the 1960s has led to the development of many rheological models, but the predictions from these models are not entirely consistent with observations.

In this work, I will consider the motion of sea ice at three different scales: (i) floe-scale or `microscopic'; (ii) mesoscopic; and (iii) continuum. Starting from the dynamics at the scale of an individual ice floe I will obtain the continuum equations by coarse graining. This approach is similar to the one used to obtain the Navier-Stokes equation from the Boltzmann equation, and allows for the determination of shear viscosity of the ice cover as an explicit function of ice concentration and mean thickness. I will compare results from the theory with observations and idealised simulations and also discuss a more general approach that accounts for phase change and mechanical deformation of ice floes.

How to cite: Toppaladoddi, S.: Sea ice motion on multiple scales, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13703, https://doi.org/10.5194/egusphere-egu26-13703, 2026.

EGU26-14157 | Orals | NP1.1

A generalisation of the signal-to-noise ratio using proper scoring rules 

Jochen Broecker and Eviatar Bach

A signal-to-noise "paradox" was first described in the context of ensemble forecasts on seasonal timescales. It refers to a situation in which the correlation between the ensemble mean and the actual verification is larger than the correlation between the ensemble mean and individual ensemble members. A noted problem of the signal-to-noise paradox remains that the signal-to-noise ratio itself, or equivalently the ratio of predictable components (RPC), which are used to diagnose the signal-to-noise paradox, has poorly understood statistical properties, rendering reliable identification of the signal-to-noise paradox difficult.

In this contribution, a generalised concept of the RPC is discussed based on proper scoring rules. This definition is the natural generalisation of the classical RPC, yet it allows one to define and analyse the signal-to-noise properties of any type of forecast that is amenable to scoring, thus drastically widening the applicability of these concepts. The methodology is illustrated for ensemble forecasts, scored using the continuous ranked probability score (CRPS), and for probability forecasts of a binary event, scored using the logarithmic score. Numerical examples demonstrate that the classical and new RPC statistic agree regarding which data sets exhibit anomalous signal-to-noise ratios, but exhibit different variance, indicating different statistical properties.

How to cite: Broecker, J. and Bach, E.: A generalisation of the signal-to-noise ratio using proper scoring rules, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14157, https://doi.org/10.5194/egusphere-egu26-14157, 2026.

EGU26-14650 | ECS | Orals | NP1.1

Comparing Rare-Event Algorithms and Direct Sampling for Estimating the Probability of CO₂-Driven AMOC Tipping 

Matteo Cini, Valerian Jacques-Dumas, Giuseppe Zappa, Francesco Ragone, and Henk A. Dijkstra

The Atlantic Meridional Overturning Circulation (AMOC) is a key tipping element of the climate system and can be viewed as a multistable, stochastic dynamical system subject to both external forcing and internal variability. While most modelling studies emphasize deterministic thresholds for AMOC collapse, the role of internal variability in shaping the timing, probability, and nature of transitions remains poorly constrained.

This motivates a shift toward probabilistic prediction of AMOC tipping. Transition probabilities can be estimated using direct Monte Carlo sampling with large ensembles; however, this approach is severely limited in climate applications, as simulations are computationally expensive and statistical precision improves only slowly with increasing ensemble size. Rare-event algorithms provide an efficient alternative. In particular, the Giardina–Kurchan–Tailleur–Lecomte (GKTL) and Trajectory-Adaptive Multilevel Splitting (TAMS) methods enable targeted sampling of low-probability transitions at substantially reduced computational cost.

Using the intermediate-complexity PlaSIM–LSG model, we estimate AMOC transition probabilities by comparing direct Monte Carlo sampling with GKTL and TAMS. In a 600 ppm CO₂ case study, TAMS delivers the most precise probability estimates per unit cost, outperforming both Monte Carlo and GKTL and emerging as the most reliable approach for probability estimation.

We further apply TAMS to assess the transition probability to a weak AMOC state under three SSP scenarios, revealing a strong dependence on the forcing pathway. Under the high-emissions scenario SSP5–8.5, the probability of entering the AMOC-weak state remains below 1% by 2100, increases to about 20% by 2150, and reaches roughly 95% by 2200. In contrast, lower-emission scenarios (SSP4–6.0 and SSP2–4.5) maintain substantially lower probabilities throughout. These results are consistent with recent multi-model projections, suggesting that AMOC collapse is very unlikely in the 21st century but becomes plausible in the 22nd century under sustained high forcing. Additional freshwater input from Greenland ice-sheet melt would likely further increase these probabilities and advance the transition.

Overall, when direct sampling fails to capture rare transitions, rare-event methods enable both improved probability estimation and deeper insight into the underlying physical mechanisms. GKTL is well suited for exploring multistability and multiple transitions, while TAMS provides a rigorous framework for quantifying transition probabilities. Together, these approaches help bridge the gap between theoretical concepts of multistability and their practical investigation in complex climate models.

How to cite: Cini, M., Jacques-Dumas, V., Zappa, G., Ragone, F., and Dijkstra, H. A.: Comparing Rare-Event Algorithms and Direct Sampling for Estimating the Probability of CO₂-Driven AMOC Tipping, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14650, https://doi.org/10.5194/egusphere-egu26-14650, 2026.

EGU26-15666 | ECS | Orals | NP1.1

Data-driven identification of atmospheric drivers of anomalous Antarctic sea ice loss 

Courtney Quinn, Andrew Axelsen, Terence O'Kane, and Andrew Bassom

Over the past decade there have been unprecedented events of record low sea ice concentration in the Antarctic region. Previous work has attributed these anomalous sea ice loss events to persistent anomalies in various atmospheric drivers such as the Southern Annular Mode (SAM), the Pacific South American (PSA) patterns, and the Amundsen Sea Low (ASL). The majority of such studies employ methodologies that either assume stationarity or use averages over uniform fixed periods (e.g. months). In this study we show how a machine learning method applied to multiscale climate data can extract drivers across subsystems without predefining patterns or time periods. Specifically, we employ a nonstationary data-clustering framework to coupled sea ice and atmosphere reanalysis data to extract persistent coherent events across both systems. We use time-varying Markov transition matrices to extract the dominant states over a sliding time window and identify persistence as an uninterrupted period of a dominant state for at least ten days.

Analysing three years consisting of anomalously low sea ice events, we find that our approach identifies a variety of atmospheric drivers for these events without preconditioning. The dominant drivers vary in spatial extent and duration, as opposed to many stationary methods which require an a priori selection of scales. Here each event’s spatial and temporal boundaries are determined by the optimal model itself. This nonstationary analysis is thus particularly valuable for characterizing multiscale interactions and addressing dynamics across coupled climate subsystems.

How to cite: Quinn, C., Axelsen, A., O'Kane, T., and Bassom, A.: Data-driven identification of atmospheric drivers of anomalous Antarctic sea ice loss, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15666, https://doi.org/10.5194/egusphere-egu26-15666, 2026.

Accurate subsurface parameter estimation remains challenging due to the inherent nonlinearity and non-uniqueness of geophysical inverse problems. In this study, we present an integrated Bayesian–Gauss–Newton inversion framework for Electrical Resistivity Tomography (ERT) aimed at achieving robust model parameter estimation and uncertainty quantification. The Bayesian component provides a probabilistic description of the inverse problem, enabling the incorporation of prior geological information and the assessment of posterior parameter distributions. Bayesian optimization is employed to efficiently explore the high-dimensional model space and obtain a geologically consistent initial model. Subsequently, a Gauss–Newton optimization scheme is applied to refine this solution and obtain the maximum a posteriori estimate with improved convergence characteristics. The combined approach leverages the global search capability of Bayesian optimization and the computational efficiency of the Gauss–Newton method, resulting in enhanced resolution of sharp resistivity contrasts and reduced ambiguity in subsurface models. Applications to both synthetic and field ERT datasets demonstrate that the proposed methodology improves data fitting, stabilizes inversion results, and provides a comprehensive measure of model uncertainty. The results highlight the potential of the Bayesian–Gauss–Newton framework as a reliable and efficient inversion strategy for ERT-based subsurface characterization, particularly in complex environments affected by strong resistivity contrasts and saline intrusion.

How to cite: Sarkar, K. and Singh, A.: A Bayesian–Gauss–Newton Inversion Framework for Electrical Resistivity Tomography with Improved Parameter Estimation and Uncertainty Quantification, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15971, https://doi.org/10.5194/egusphere-egu26-15971, 2026.

The albedo contrast between sea ice and open ocean introduces a strong positive feedback in the surface energy balance of polar regions. Classical low-order models show that this feedback robustly produces multiple equilibria: the system can exist in either a cold, ice-covered state or a warm, ice-free state with the same external forcing.  The resulting hysteresis implies that polar regions will lose sea ice abruptly and irreversibly as external forcing increases. However, this tipping-point behavior is not observed in full-complexity climate models: in experiments where global radiative forcing is gradually ramped up until sea ice disappears, ice loss is indeed found to be relatively abrupt; but when the forcing is subsequently ramped down, sea ice reappears at the same rate, showing no sign of hysteresis or irreversibility. How do we reconcile this discrepancy between simple and complex models?

Here, I show that this reconciliation can be achieved by introducing atmospheric weather noise into the simple model. The polar ocean is modelled as a collection of points subject to local stochastic forcing, introduced as an additive white noise in the  energy balance model. This leads to a Fokker-Planck equation describing the probability distribution function (PDF) of ice thickness over the ocean basin, including a zero-thickness (ice free) class. For realistic values of noise amplitude estimated from reanalysis data, the PDF is bimodal when the global forcing supports multiple equilibria of the energy balance equation, with modes centered on the corresponding ice-free and ice covered equilibria. When global forcing is ramped up or down over long (~1000 year) timescales, the PDF evolves reversibly, showing relatively abrupt but reversible loss/recovery of sea ice. However, if the ramping timescale is shorter (~100 years), some residual irreversibility is still present. In conclusion, taking stochastic atmospheric fluctuations into account provides a promising avenue for resolving a long-standing problem in climate science.

How to cite: Caballero, R.: Atmospheric noise removes sea-ice tipping points in a simple stochastic model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17941, https://doi.org/10.5194/egusphere-egu26-17941, 2026.

EGU26-19315 | ECS | Posters on site | NP1.1

Detecting Rapid Changes and Tipping Points in the Abyssal Ocean Circulation via Deep Learning and Satellite Observations 

Arianna Ferrotti, Alberto Naveira Garabato, Alessandro Silvano, Chao Zheng, and Adele Morrison

The transport of Antarctic Bottom Water (AABW) supplies the densest layers of the abyssal ocean circulation, which accounts for up to 40% of the ocean's volume and plays a vital role in Earth's climate. Due to its recently ventilated nature, AABW carries heat and carbon from the surface to the deep ocean, allowing these elements to be isolated for centuries, while also gathering oxygen and delivering it to the ocean's depths. AABW forms when dense, cold waters from the continental shelves descend along the Antarctic slope. The physical conditions necessary for sinking are created by ice formation and freezing winds in this region.

This implies that, as temperatures rise and ice melts due to climate change, the circulation could diminish. Model projections also suggest this, identifying meltwater forcing as a potential primary factor in the reduction of AABW transport. However, the variability of AABW remains poorly constrained by observations. Its origin on the Antarctic continental shelf and slope presents limited opportunities for in situ measurements, and satellite observations are hindered, especially in winter, due to sea ice cover. Further north, AABW spreads approximately 2 km below the surface, making it difficult to monitor directly by satellites, with in situ measurements remaining scarce.

Here, we explore the plausibility of inferring AABW circulation from available satellite measurements of the ocean's surface properties, via machine learning techniques. Our work is focused on implementing a Deep Neural Network (DNN) with high skill and potential for reconstructing the circulation's strength. Different architectures are trained and tested on the ACCESS-OM2-01 model, and a cross-training with other ocean models is investigated, as well as the use of real satellite measurements and change-point detection techniques.
These studies offer a valuable means to overcome current limitations on Southern Ocean and abyssal circulation research, making it more accessible, sustainable, and consistent.

How to cite: Ferrotti, A., Naveira Garabato, A., Silvano, A., Zheng, C., and Morrison, A.: Detecting Rapid Changes and Tipping Points in the Abyssal Ocean Circulation via Deep Learning and Satellite Observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19315, https://doi.org/10.5194/egusphere-egu26-19315, 2026.

EGU26-19518 | ECS | Orals | NP1.1

Breaking of stationarity by intermittency in coupled dynamics 

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

Intermittent dynamics are a common feature of many Earth-system components that often interact across ample ranges of temporal and spatial scales.  Our previous work shed light on the mechanism driving intermittency and identified precursors of its onset (Barone et al., 2025). This current study moves forward, and it investigates the processes by which an intermittent component in a coupled system influences other ones that, in the absence of the coupling, would evolve quasi stationarily. In particular, we investigate a prototypical fast–slow, e.g. atmosphere-ocean, setup in which fast intermittent systems act as a unidirectional forcing on slow components characterized by a stable limit cycle.

Using a two-scale version of the Lorenz–63 model, we show that intermittent bursts in the fast dynamics induce deviations from the slow dynamics’s limit cycle, which, depending on the strength of the coupling and the timescale difference, can even fully destabilize the limit cycle and lead to a chaotic regime. We show that increasing the frequency of intermittent events does not necessarily affect the slow component response, which below a critical value retains its structural properties, highlighting the non-trivial nature of intermittent information transfer across scales. The induced transition from periodicity to chaos caused by the intermittent burst, is looked through the lens of the power spectrum decomposition (PSD) of the finite-time Lyapunov exponents, offering a unique view on the progressive loss of predictability in the slow component. The analysis is then extended to a spatially extended system based on unidirectionally coupled Kuramoto–Sivashinsky equations. As the coupling strength increases, the energy PSD of the slow and initially regular dynamics, progressively approaches that of the fast intermittent system, up to a regime in which the two become effectively indistinguishable. Remarkably, mutual information between subsystems reveals a clear latency in the slow response that increases with the degree of time-scale separation.

Our study provides a robust framework to investigate similar dynamical configurations in Earth system models, whereby a fast intermittent atmosphere induces short-living, yet impactful, changes in a slow ocean. 

A. Barone, A. Carrassi, T. Savary, J. Demaeyer, S. Vannitsem; Structural origins and real-time predictors of intermittency. Chaos 1 October 2025; 35 (10): 103119. https://doi.org/10.1063/5.0287572

How to cite: Barone, A., Carrassi, A., Demaeyer, J., and Vannitsem, S.: Breaking of stationarity by intermittency in coupled dynamics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19518, https://doi.org/10.5194/egusphere-egu26-19518, 2026.

EGU26-19654 | ECS | Posters on site | NP1.1

A Linear State-Space Model of the Lorenz-63 System and Its Applications 

Pak Wah Chan, Yutian Hou, Xingfeng Li, Juejin Wei, Junwei Chen, and Ding Ma

The climate is a nonlinear system, but it is sometimes useful to approximate it as a linear system.  Considering the climate response under steady forcing (e.g., heating tendency), a linear Markov model (a model without memory effect) should never give a response opposite to the forcing, because it implies an unstable mode.  Here, using the Lorenz-63 system, a 3-variable nonlinear system simplified from 2D convection, as testbed, we show that the climate response of a nonlinear system can be exactly opposite to the forcing, demonstrating a shortcoming of linear Markov model which cannot tolerate an opposite response.  Such opposite response arises not from numerical errors nor reduction of prognostic variables, as previously suggested.  We build a linear state-space model (SSM, a model with memory effect) and quantitatively explain how memory effect gives rise to an opposite response.  Our linear SSM can serve as a benchmark in a unified testbed, where other indirect methods to compute climate response, e.g., fluctuation-dissipation theorem (FDT), can be examined and refined.  Our linear SSM can also be applied to accurately predict response under periodic forcing.  With this, the resonant frequencies of the system can be identified.  The Lorenz-63 system may be far from real world.  Yet, the same approach can be applied to quantitatively analyze the dynamics of natural variability of the climate system, such as annular mode.

Published/submitted:

Hou, Y., Chen, J., Ma, D., & Chan, P. W. (2025). Steady-state linear response matrix of the Lorenz-63 system. J. Atmos. Sci., 82(12), 2667-2675. https://doi.org/10.1175/JAS-D-25-0016.1

Hou, Y., & Chan, P. W. (submitted). A linear state-space model of the Lorenz-63 system and its applications. https://doi.org/10.6084/m9.figshare.30271819.v1

How to cite: Chan, P. W., Hou, Y., Li, X., Wei, J., Chen, J., and Ma, D.: A Linear State-Space Model of the Lorenz-63 System and Its Applications, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19654, https://doi.org/10.5194/egusphere-egu26-19654, 2026.

EGU26-21740 | ECS | Orals | NP1.1

Evaluation of data assimilation methods suitable for frontal structures 

Saori Nakashita and Takeshi Enomoto

Frontal structures, frequently observed in the vicinity of westerly jets and western boundary currents, are characterized by sharp gradients in both horizontal and vertical directions. Forecast errors associated with these fronts often exhibit non-Gaussian distributions due to biases in frontal location or magnitude stemming from sparse observation networks or misrepresented model physics. Such non-Gaussianity poses significant challenges for conventional data assimilation (DA) schemes that rely on Gaussian assumptions.
In this study, we investigate the performance of various ensemble DA methods in representing fronts using idealized simulations with a frontogenesis model (Keyser et al., 1988). The compared methods include the stochastic Ensemble Kalman Filter (EnKF), the Ensemble Adjustment Kalman Filter (EAKF), and the Nonlinear Ensemble Transform Filter (NETF). Furthermore, we propose a novel nonlinear DA approach termed the Kernelized EAKF (KEAKF). By integrating kernel ridge regression into the EAKF framework, KEAKF effectively accounts for nonlinear relationships between state variables.
To simulate realistic forecast biases, the first-guess ensembles are initialized with systematic errors in both frontal magnitude and location. DA performance is rigorously evaluated using three metrics: root mean squared error (RMSE) of temperature (state error), RMSE of the temperature gradient (magnitude error), and the modified Hausdorff distance of frontal locations (displacement error). Our results demonstrate that KEAKF outperforms all other methods across all evaluation metrics. While the EnKF shows relatively stable performance in state estimation, the EAKF is superior in capturing frontal magnitude and location. The NETF, despite its non-Gaussian formulation, shows limited performance due to particle degeneracy in this setting. Finally, we discuss the implications of these findings for maintaining dynamical balances and improving the predictability of frontal systems in more complex dynamical models.

How to cite: Nakashita, S. and Enomoto, T.: Evaluation of data assimilation methods suitable for frontal structures, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21740, https://doi.org/10.5194/egusphere-egu26-21740, 2026.

EGU26-22041 | Orals | NP1.1

The Parallel Data Assimilation Framework (PDAF) - Upgrade to Version 3 

Lars Nerger, Yumeng Chen, Armin Corbin, and Johannes Keller

PDAF is open-source software (https://pdaf.awi.de) providing a unified data assimilation framework for all data assimilation applications throughout the Earth system and beyond. PDAF is already coupled to a wide range of models, including all Earth system components, and is widely used for research and operational applications. With well-defined interfaces and modularization motivated by object-oriented programming, PDAF separates the forecast model, the observation handling, and the data assimilation algorithms. This structure ensures separation of concerns and allows domain experts to perform further developments of each component independently without interfering with each other. PDAF is further designed to make the coupling to models, online in memory or offline using disk files, particularly easy so that a new assimilation system can be built quickly. 
PDAF was recently upgraded to the new major revision 3.0. In PDAF V3, the code was modernized and restructured simplifying the procedure to add further data assimilation algorithms. New features are supported including model-agnostic incremental analysis updates, new diagnostics for observations and ensembles, and the ensemble square root filter (EnsRF) and ensemble adjustment Kalman filter (EAKF). With this, PDAF now provides the full range of algorithms from domain-localized ensemble filters and smoothers to Kalman filters with serial observation processing, particle and hybrid Kalman-nonlinear filters, and 3-dimensional variational data assimilation methods. Existing users can switch to PDAF V3 with minimal effort, while a new universal interface supporting all filters is recommended for new users. The Python-interface, pyPDAF, further allows the full implementation of an assimilation program in Python, leveraging the functionality and performance provided by PDAF. We will provide an overview of PDAF and the novelties of version 3.0.

How to cite: Nerger, L., Chen, Y., Corbin, A., and Keller, J.: The Parallel Data Assimilation Framework (PDAF) - Upgrade to Version 3, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22041, https://doi.org/10.5194/egusphere-egu26-22041, 2026.

EGU26-22978 | Orals | NP1.1

Modelling of Southern Ocean decadal variability arising from eddy-mean interactions 

Julian Mak, Han Seul Lee, James Maddison, David Marshall, Yan Wang, and Yue Wu

The Southern Ocean is an important component of the Earth climate system through its role in regulating and impacting the global ocean circulation. The Southern Ocean is known to be strongly turbulent, and that eddies play a role in regulating the mean and vice-versa. It is of interest to understand and model the resulting internal variability arising from such eddy-mean interactions, from a theoretical point of view because it provides further understanding to strongly interacting fluid systems, but also in practical terms because such internal variability is present in eddy-present/rich models but not so in coarse resolution parameterised models, which has consequences for example for anthropogenic carbon uptake. Here a low-order dynamical systems model of the eddy-mean interaction is constructed/derived, bearing resemblance to nonlinear oscillator and/or predator-prey type models of storm-tracks in the atmosphere and those in plasma physics for zonal-flow/drift-wave turbulence. Oscillatory time-scales for the model are derived, and testing is done on whether the derived time-scales are present in a hierarchy of numerical ocean models ranging from layered models to a primitive equation sector model. Evidence is presented that the GEOMETRIC parameterisation for geostrophic mesoscale eddies may improve the representation of decadal variability in the Southern Ocean, potentially leading to impacts in the modelled ventilation of oxygen and anthropogenic carbon in the Southern Ocean.

How to cite: Mak, J., Lee, H. S., Maddison, J., Marshall, D., Wang, Y., and Wu, Y.: Modelling of Southern Ocean decadal variability arising from eddy-mean interactions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22978, https://doi.org/10.5194/egusphere-egu26-22978, 2026.

EGU26-2310 | ECS | Posters on site | NP1.2

Reduced Complexity Model Intercomparison Project Phase 3: protocol and preliminary results 

Alejandro Romero-Prieto, Marit Sandstad, Benjamin M. Sanderson, Zebedee R. J. Nicholls, Norman J. Steinert, Thomas Gasser, Camilla Mathison, Jarmo Kikstra, Thomas J. Aubry, Katsumasa Tanaka, Konstantin Weber, and Chris Smith

Reduced-complexity models (RCMs) are a critical tool in climate science. Their computational efficiency enables applications beyond the reach of more complex models, including uncertainty quantification, the integration of multiple lines of evidence via ensemble constraining, and running large scenario sets in the span of a few days. Thanks to these capabilities, RCMs played important roles in previous IPCC assessments, and are poised to play an important role in the upcoming Seventh Assessment Report (AR7). A key example is evaluating the climate response to the thousands of emissions scenarios in the peer-reviewed literature created with integrated assessment models. However, whether/which RCMs are suitable for performing such a task is contingent on their ability to faithfully emulate the behaviour of more complex models and observed climate change.

The Reduced-Complexity Model Intercomparison Project (RCMIP) was established to assess this capability, as well as to better understand inter-RCM differences (Nicholls et al., 2020; Nicholls et al., 2021). Here, we introduce the protocol for the third and latest phase, RCMIP3. This phase focuses on two priorities. First, it provides a common set of observational benchmarks to be optionally used for ensemble constraining prior to submission, with the objective of mitigating discrepancies arising from different calibration methodologies and facilitating a clearer assessment of intrinsic model differences. Second, it requests an expanded set of variables and experiments from modelling teams to enable a more thorough evaluation of the carbon cycle representation in these models – a key gap in previous RCMIP phases. Additionally, RCMIP3 includes many of the experiments in the “Assessment Fast Track" (AFT) of the Coupled Model Intercomparison Project Phase 7 (CMIP7). As a result, RCMIP3 will improve our understanding of future model differences under these experiments, in addition to providing the community with valuable early projections.

The presentation will outline the RCMIP3 protocol and highlight the types of analyses it enables, along with preliminary results. By explicitly comparing RCM outputs with both ESM simulations and observations, RCMIP3 aims to strengthen the linkage across the climate-model hierarchy as well as evaluating and showcasing the suitability of RCMs for climate assessment.

Nicholls, Z., Meinshausen, M., Lewis, J., Corradi, M.R., Dorheim, K., Gasser, T., Gieseke, R., Hope, A.P., Leach, N.J., McBride, L.A., Quilcaille, Y., Rogelj, J., Salawitch, R.J., Samset, B.H., Sandstad, M., Shiklomanov, A., Skeie, R.B., Smith, C.J., Smith, S.J., Su, X., Tsutsui, J., Vega-Westhoff, B. and Woodard, D.L. 2021. Reduced Complexity Model Intercomparison Project Phase 2: Synthesizing Earth System Knowledge for Probabilistic Climate Projections. Earth’s Future. 9(6), https://doi.org/10.1029/2020EF001900.

Nicholls, Z.R.J., Meinshausen, M., Lewis, J., Gieseke, R., Dommenget, D., Dorheim, K., Fan, C.-S., Fuglestvedt, J.S., Gasser, T., Golüke, U., Goodwin, P., Hartin, C., Hope, A.P., Kriegler, E., Leach, N.J., Marchegiani, D., McBride, L.A., Quilcaille, Y., Rogelj, J., Salawitch, R.J., Samset, B.H., Sandstad, M., Shiklomanov, A.N., Skeie, R.B., Smith, C.J., Smith, S., Tanaka, K., Tsutsui, J. and Xie, Z. 2020. Reduced Complexity Model Intercomparison Project Phase 1: introduction and evaluation of global-mean temperature response. Geoscientific Model Development. 13(11), pp.5175–5190, https://doi.org/10.5194/gmd-13-5175-2020.

How to cite: Romero-Prieto, A., Sandstad, M., Sanderson, B. M., Nicholls, Z. R. J., Steinert, N. J., Gasser, T., Mathison, C., Kikstra, J., Aubry, T. J., Tanaka, K., Weber, K., and Smith, C.: Reduced Complexity Model Intercomparison Project Phase 3: protocol and preliminary results, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2310, https://doi.org/10.5194/egusphere-egu26-2310, 2026.

EGU26-4264 | Posters on site | NP1.2

METEOR 1.5 a spatial emulator for fast and relevant responses to impact questions 

Marit Sandstad, Benjamin Sanderson, Norman Steinert, and Shivika Mittal

Here we present an extended version of the forcing-driven and overshoot-aware spatial impacts emulator METEOR, which now includes functionality to emulate monthly outputs which include seasonality and natural variability, with the option to produce large distribution ensembles for a point, regional average or spatial domain.  The philosophy of METEOR entails fast training on few and widely available datasets, sufficiently fast to be run on-the-fly and removing the need to archive large datasets and allowing interactive coupling with integrated assessment frameworks to simulate impacts directly.  METEOR1.5 introduces a state dependent seasonal model and an autoregressive spatial, state-dependent noise model which can produce distributions of realisations conforming to the climatic trends and distributional properties of the emulated model    Integrated impact modules allow the direct emulation of human and ecological stressors which are computed from easily retrained emulated climates to answer regional questions. 

How to cite: Sandstad, M., Sanderson, B., Steinert, N., and Mittal, S.: METEOR 1.5 a spatial emulator for fast and relevant responses to impact questions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4264, https://doi.org/10.5194/egusphere-egu26-4264, 2026.

EGU26-5437 | ECS | Orals | NP1.2

When and where higher-resolution climate data improve impact model performance 

Johanna Malle, Christopher Reyer, and Dirk Karger and the ISIMIP modellers and sector coordinators

Climate impact assessments increasingly rely on high-resolution climate and forcing datasets, under the premise that finer detail enhances both the accuracy and the policy relevance of projections. Systematic evaluations of when and where higher resolution data improve model outcomes remain limited, and it is still unclear whether increasing spatial resolution consistently enhances climate impact model performance across application areas, regions, and forcing variables. Here we show that improvements in climate input accuracy and impact model performance are most pronounced when moving from coarse (60 km) to intermediate (10 km) resolution, while further refinement to 3 km and 1 km provides more modest and inconsistent benefits. Using the cross-sectoral model simulations from the Inter-Sectoral Impact Model Intercomparison Project (ISIMIP), we demonstrate that higher resolution substantially improves model skill in temperature-sensitive impact models and topographically complex regions, whereas precipitation-driven and low-relief systems show less consistency to increase performance with resolution. For temperature, both climate inputs and model outputs improved most strongly at the 60 km → 10 km transition, with diminishing gains at finer scales. A similar result emerged for precipitation, although some models even exhibited reduced performance when resolution increased beyond 10 km. These results highlight that optimal resolution depends on sectoral and regional context, and point to the need for improving model process representation and downscaling techniques so that added spatial detail can translate into meaningful performance gains. For data providers, this implies prioritizing investments in resolutions that maximize improvements where they matter most, while for modeling groups and users, it underscores the need for explicit benchmarking of resolution choices. More broadly, this work advances the design of consistent, efficient, and policy-relevant multi-sectoral climate impact assessments by clarifying when high-resolution data meaningfully enhance outcomes.

How to cite: Malle, J., Reyer, C., and Karger, D. and the ISIMIP modellers and sector coordinators: When and where higher-resolution climate data improve impact model performance, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5437, https://doi.org/10.5194/egusphere-egu26-5437, 2026.

EGU26-5816 | ECS | Posters on site | NP1.2

Defining an early warning method for an AMOC collapse based on ensemble statistics 

Dániel Jánosi, Ferenc Tamás Divinszki, Reyk Börner, and Mátyás Herein

The Atlantic Meridional Overturning Circulation (AMOC) is a crucial climate component, as its potential collapse would constitute a significant response to Earth’s changing climate. This critical transition has been the subject of numerous studies over the years, both from the aspect of climate modeling and dynamical systems theory. In the context of the latter, climate change is a process in which a complex, chaotic-like system possesses time-dependent parameters, in the form of e.g. the growing CO2 concentration. It has been known that such systems have a chaotic attractor which is also time-dependent, a so-called snapshot attractor. Such objects, and thus the systems they describe, can only be faithfully represented by a probability distribution over an ensemble of simulations, so-called parallel climate realizations.

Based on this probability distribution, we define a novel early warning indicator for crucial transitions such as an AMOC collapse. The AMOC is said to possess a multistable quasipotential landscape, and the collapse is a transition between stable states. We argue that, from the point of view of statistical physics, this is analogous to a phase transition, but in a non-adiabatic setting. As such, the variance of the distribution over the ensemble is expected to develop a local maximum around the transition point, giving rise to a potential early warning by identifying the preceding maximum of its derivative. This method is first demonstrated on a conceptual climate model, before the analysis is carried out on ensemble simulations from the ACCESS-ESM model. The analysis in the former case is simpler, while in the latter, one has to contend with the dependence of the AMOC strength on spatial coordinates, resulting in multiple early warning points for different depths and latitudes.

How to cite: Jánosi, D., Divinszki, F. T., Börner, R., and Herein, M.: Defining an early warning method for an AMOC collapse based on ensemble statistics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5816, https://doi.org/10.5194/egusphere-egu26-5816, 2026.

Offline aridity and drought indices have often implied widespread terrestrial drying under a warming environment, while Earth system models (ESMs) have projected modest changes in land-surface water fluxes. This persistent divergence has been typically attributed to missing vegetation physiological processes in offline frameworks. However, we here show that a more foundational cause is a structural inconsistency embedded in those diagnostics. Conventional potential evapotranspiration (PET) formulations can violate the assumption that precipitation (P) and atmospheric evaporative demand act as independent climatic constraints in the Budyko framework. Using open-water Penman and vegetation-responsive Penman–Monteith formulations forced by reanalysis data and ESM projections, we found that uncorrected PET strongly reflected land–atmosphere feedbacks, leading to pronounced negative P–PET correlations (-0.45 ± 0.29; mean ± s.d.). When PET was thermodynamically deflated, this dependence was largely removed (-0.02 ± 0.42), restoring consistency with the theoretical basis of Budyko-type diagnostics. This structural correction reduced inflation of the aridity index and substantially moderated projected evapotranspiration (ET) trends. Under a business-as-usual scenario, the trend of Budyko-based ET from uncorrected PET (+0.61 mm yr-2) exceeded that of CMIP6 ensemble mean (+0.28 mm yr-2) by more than a factor of two. CEP-deflated PET narrowed this discrepancy (+0.39 mm yr-2), while additional physiological adjustments provided comparatively smaller improvements. We suggest that violations of structural assumptions, rather than missing physiological processes alone, can play a central role in the divergence between offline aridity diagnostics and ESM hydrological projections.

Acknowledgement: This work was jointly supported by the National Research Foundation of Korea (NRF) grants funded by the Korea government (MSIT) (RS-2025-16070291 & RS-2024-00416443).

How to cite: Kim, D. and Choi, M.: Why offline aridity diagnostics overestimate future drying: the role of feedback-inflated evaporative demand, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6189, https://doi.org/10.5194/egusphere-egu26-6189, 2026.

EGU26-6930 | ECS | Posters on site | NP1.2

Barotropic waves in a sloping two- and multiple-basin Arctic ocean model 

Michael Duc Tung Nguyen and Edward Johnson

Large-scale barotropic flow in the Arctic Ocean is strongly steered by the seafloor topography, yet how this geometry constrains free modes and facilitates inter-basin interactions remains unclear. Free modes conserve potential vorticity and at high latitudes the circulation pathway is enclosed by its sloping two-basin geometry. We begin by presenting a simple two-basin model, representing the Canadian and Eurasian basin respectively, with sloping boundaries and flat bottoms to explore simplified Arctic flow behaviour. Topographic Rossby waves are analytically obtained and the two basins are linked together via a mode-matching framework. We show free modes are tightly constrained to geometry, with basin-trapped dipole wave modes only emerging in certain geometric parameters. We then extend this to a more realistic, multiple-basin Arctic Ocean model that include the Nordic seas, and demonstrate the transmission and exchange of these topographic waves across these multiple sloping basins.

How to cite: Nguyen, M. D. T. and Johnson, E.: Barotropic waves in a sloping two- and multiple-basin Arctic ocean model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6930, https://doi.org/10.5194/egusphere-egu26-6930, 2026.

EGU26-7143 | ECS | Posters on site | NP1.2

Jax-esm: a differentiable coupler for jax-based Earth system models 

Tien-Yiao Hsu, Duncan Watson-Parris, and Georg Feulner

The differentiability of numerical climate models exhibits  many advantages over non-differentiable models. Differentiable climate models would be able to optimize parameters and quickly solve for climate equilibrium. They can also be used to find unstable climate equilibrium states that are impossible to identify in time-forwarding models. Differentiability also enables sensitivity studies, such as the impact of initial conditions on predictions, which is the key concept in the 4-dimensional variational method. Finally, differentiable ability also integrates well with the trending data-driven artificial intelligence model, such as NeuralGCM.  

Currently, physics-based differentiable coupled climate models are still rare. Some existing ones include: ECMWF Integrated Forecasting System (ECMWF-IFS) and Coupled Ocean/Atmosphere Mesoscale Prediction System (COAMPS). The high scientific value of such a tool warrants development of further differentiable modelling systems.

In this work, we present jax-esm, a differentiable coupler for models written in Python with the JAX framework. JAX is a Python library developed by Google that builds on NumPy and adds automatic differentiation and just-in-time (JIT) compilation. It has been used to develop atmospheric models such as NeuralGCM and jax-gcm. In this example, we couple jax-gcm, a JAX-based atmosphere intermediate model, to a slab ocean model. We demonstrate the optimization of ocean mixed-layer depth and solving for climate equilibrium through differentiability.

How to cite: Hsu, T.-Y., Watson-Parris, D., and Feulner, G.: Jax-esm: a differentiable coupler for jax-based Earth system models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7143, https://doi.org/10.5194/egusphere-egu26-7143, 2026.

EGU26-7983 | ECS | Posters on site | NP1.2

Multi-stability of the Global Overturning Circulation: A Conceptual Approach 

Elian Vanderborght and Henk Dijkstra

The Global Overturning Circulation (GOC) is characterized by deep water formation in the subpolar North Atlantic, which feeds the southward-flowing branch of the Atlantic Meridional Overturning Circulation (AMOC). In contrast, the North Pacific lacks deep water formation and therefore does not host an analogous Pacific Meridional Overturning Circulation (PMOC). Proxy records, however, indicate that this asymmetric pattern of deep water formation has varied in the past, suggesting that a PMOC likely existed during earlier climate states. Recent studies further show that the development of a PMOC influences the future weakening of the AMOC: climate models that develop a PMOC in response to warming exhibit a stronger decline in AMOC strength. It therefore becomes important to understand under what circumstances a PMOC is likely to develop.

Here, we extend the pycnocline model of Gnanadesikan (1999) to a two-basin configuration, consisting of a narrow basin representing the Atlantic and a wide basin representing the Pacific. By including salinity as a prognostic variable, we find that this two-basin box model may exhibit three distinct overturning states under identical, longitudinally symmetric forcing: (1) an active narrow-basin sinking state, (2) an active wide-basin sinking state, and (3) a state with active sinking in both basins. Overturning states confined to a single basin are stabilized by the salt-advection feedback, whereas the state with sinking in both basins is maintained by a meridional temperature contrast. We find that this latter state becomes the preferred equilibrium when the interhemispheric temperature contrast increases, the northern gyre transport strengthens, and the hydrological cycle weakens. Moreover, we show that this state is more sensitive to high-latitude freshwater fluxes, indicating that a transition to such a state would enhance the projected future weakening of the AMOC. We verify these findings in an uncoupled global circulation model (MITgcm) with a simplified model geometry.

How to cite: Vanderborght, E. and Dijkstra, H.: Multi-stability of the Global Overturning Circulation: A Conceptual Approach, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7983, https://doi.org/10.5194/egusphere-egu26-7983, 2026.

EGU26-8370 | ECS | Posters on site | NP1.2

Quantifying AMOC Uncertainty in European Climate Damage Projections 

Felix Schaumann

Estimates of economic damages from climate change in Europe depend on temperature projections, and they are thereby subject to scenario uncertainty and model uncertainty, as well as damage function uncertainty. An additional, often implicit source of uncertainty is the projected, yet poorly constrained, weakening of the Atlantic Meridional Overturning Circulation (AMOC), which would lower European temperatures. Here, I explicitly quantify the contribution of AMOC uncertainty to total damage uncertainty, with AMOC uncertainty comprising uncertainty about future AMOC developments as well as uncertainty about the cooling pattern that would follow an AMOC weakening. I combine a newly developed pattern-scaling-type emulator of the European cooling response to AMOC weakening — calibrated for different Earth system models (ESMs) — with temperature projections from multiple ESMs and emissions scenarios, alongside several damage functions. This allows me to decompose the total uncertainty in European economic damages into different drivers and estimate the share attributable to the behaviour of the AMOC.

How to cite: Schaumann, F.: Quantifying AMOC Uncertainty in European Climate Damage Projections, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8370, https://doi.org/10.5194/egusphere-egu26-8370, 2026.

The history of climate modelling is one of increasing complexity and increasing resolution, driven by and constrained by the available computational capacity. These models are widely used, directly and indirectly, to support policy and adaptation decisions across society. They are also used in academic studies across a range of disciplines to study the response of the climate system to future atmospheric greenhouse gas concentrations on multi-decadal timescales. These are extrapolatory endeavours in a non-stationary system without possibility of relevant verification.

There has been much research on individual and multi-model analyses in this context. Here I will instead discuss how the targets of our endeavours (particularly the support of societal decisions) demands a rethinking of our modelling activities. I will highlight the need to reflect on the minimum requirements for ensemble size and ensemble variety, and the role of a hierarchy of models in providing the best possible information to stakeholders across society.

These issues will be discussed in the light of a recent meeting on the foundations of climate change science attended by over 70 researchers across a variety of disciplines. The meeting was entitled “How to spend 15 billion dollars?: A workshop on how to make climate change modelling more robust and more useful to society.” It gathered expertise from disciplines as diverse as earth system modelling, integrated assessment modelling, philosophy, economics, maths, statistics and finance.

Here I will present the key messages coming out of this meeting alongside the themes presented in a recent essay on the subject, “A Model of Catastrophe”[1].

[1] Stainforth, D.A., “A Model of Catastrophe”, Aeon.co, 2025 (https://aeon.co/essays/todays-complex-climate-models-arent-equivalent-to-reality)

How to cite: Stainforth, D.: Designing Climate Change Modelling to Support Societal Decisions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8434, https://doi.org/10.5194/egusphere-egu26-8434, 2026.

EGU26-9869 | Orals | NP1.2

Cascaded score-based emulation of Earth system models for impact evaluation with SCALES-MESH  

Verena Kain, Niklas Schwind, Annika Högner, Assaf Shmuel, Alexander Nauels, Zebedee Nicholls, Marco Zecchetto, and Carl-Friedrich Schleussner

Today's climate adaptation and mitigation planning tasks require rapid access to large ensembles of climate projections for a wide range of emissions scenarios, including overshoot scenarios. While Earth system models (ESMs) provide physically consistent projections, their high computational cost limits scenario exploration. Climate emulators -  statistical or machine-learning-based models trained on ESM data to generate data replicating the ESMs behaviour for a multitude of emissions scenarios - are therefore proposed to deliver these projections efficiently. Here we present the novel modular SCALES–MESH emulator framework, combining physics-based regional projections with AI downscaling capabilities. The SCALES module translates projections of global mean surface air temperature into regional surface air temperature projections aggregated over the AR6-IPCC regions, while the MESH module performs spatio-temporal downscaling to gridded fields using a conditional score-based generative model. MESH is trained on multiple datasets and evaluated against parent ESMs using spatial, temporal, and distributional diagnostics. Results show that the emulator captures regional patterns, temporal variability, and probability distributions of emulated climate variables, including during warming and cooling phases of overshoot scenarios. We further demonstrate the potential for transfer learning across ESMs, pointing toward scalable multi-model and resolution-agnostic emulation. Together, SCALES–MESH enables rapid, flexible, and physically grounded exploration of climate futures, supporting decision-relevant climate risk assessment at unprecedented scope.

How to cite: Kain, V., Schwind, N., Högner, A., Shmuel, A., Nauels, A., Nicholls, Z., Zecchetto, M., and Schleussner, C.-F.: Cascaded score-based emulation of Earth system models for impact evaluation with SCALES-MESH , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9869, https://doi.org/10.5194/egusphere-egu26-9869, 2026.

EGU26-12377 | ECS | Orals | NP1.2

Conditions for instability in the climate–carbon cycle system 

Joseph Clarke, Chris Huntingford, Paul Ritchie, Rebecca Varney, Mark Williamson, and Peter Cox

The climate and carbon cycle interact in multiple ways. An increase in carbon dioxide in the atmosphere warms the climate through the greenhouse effect, but also leads to uptake of CO2 by the land and ocean sink, a negative feedback. However, the warming associated with a CO 2 increase is also expected to suppress carbon uptake, a positive feedback. This study addresses the question: “under what circumstances could the climate–carbon cycle system become unstable?” It uses both a reduced form model of the climate–carbon cycle system as well as the complex land model JULES, combined with linear stability theory, to show that: (i) the key destabilising loop involves the increase in soil respiration with temperature; (ii) the climate–carbon system can become unstable if either the climate sensitivity to CO2 or the sensitivity of soil respiration to temperature is large, and (iii) the climate–carbon system is stabilized by land and ocean carbon sinks that increase with atmospheric CO2 , with CO2-fertilization of plant photosynthesis playing a key role. For central estimates of key parameters, the critical equilibrium climate sensitivity (ECS) that would lead to instability at current atmospheric CO2 lies between about 11K (for large CO2 fertilization) and 6K (for no CO2 fertilization). Given the apparent stability of the climate–carbon cycle, we can view these parameter combinations as implausible. The latter value is close to the highest ECS values amongst the latest Earth Systems Models. We find that the stability of the climate–carbon system increases with atmospheric CO2 , such that the glacial CO2 concentration of 190 ppmv would be unstable even for ECS greater than around 4.5 K in the absence of CO2 fertilization of land photosynthesis.

How to cite: Clarke, J., Huntingford, C., Ritchie, P., Varney, R., Williamson, M., and Cox, P.: Conditions for instability in the climate–carbon cycle system, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12377, https://doi.org/10.5194/egusphere-egu26-12377, 2026.

EGU26-12408 | ECS | Posters on site | NP1.2

Revealing Probabilistic Patterns of Climate Extremes and Impacts Through Emulator-Based Risk Analysis 

Lorenzo Pierini, Chahan Kropf, Lukas Gudmundsson, Sonia I. Seneviratne, and David N. Bresch

Traditional earth system model ensembles provide valuable information on climate extremes. However, their limited size often underrepresents rare high-impact events, restricting the ability to explore extreme outcomes and large-scale anomaly patterns. Using the climate emulator MESMER, trained on CMIP6 models, together with the risk assessment platform CLIMADA, we assess population exposure to annual maximum daily temperatures and asset exposure to annual maximum daily precipitation.

MESMER generates virtually unlimited, spatially explicit, global climate realizations for any scenario defined by emission or global-mean-temperature trajectories. This allows us to characterize the spread of potential outcomes and associated spatial patterns, identify rare high-impact realizations, compare results with standard CMIP6 ensembles, or explore custom scenarios beyond existing model experiments.

We illustrate spatial and temporal patterns of exposure for temperature and precipitation extremes, highlighting contrasting regional responses and how highly impactful outcomes can emerge from climate variability.



How to cite: Pierini, L., Kropf, C., Gudmundsson, L., Seneviratne, S. I., and Bresch, D. N.: Revealing Probabilistic Patterns of Climate Extremes and Impacts Through Emulator-Based Risk Analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12408, https://doi.org/10.5194/egusphere-egu26-12408, 2026.

EGU26-12585 | Posters on site | NP1.2

Parsimonious models emulating millennium-long Earth system model simulations 

Kristoffer Rypdal

Parsimonious emulator models (PEMs) trained on Earth system models (ESMs) can be very useful when information  about global quantities like global mean surface temperature (GMST) and ocean heat content (OHC) are sought. Here, I use data over several millennia from ESM runs extracted from the LongRunMip repository to construct and test PEMs for GMST and net incoming radiation flux.

For the  GMST, I consider a linear impulse response in the form of a superposition of three decaying exponentials, comprising three weight coefficients and three characteristic decay times to be estimated by least square fitting to ESM runs with abrupt step function forcing. The model fit is good on all time scales, and the fitted model seems to perform even better for smoother forcing scenarios. This sugggests that the six model parameters represent essential features of each ESM.

Data for radiation flux, and its decomposition in longwave and reflected shortwave, are combined with GMST to produce Gregory plots. By fitting parabolic curves to these plots, I obtain a simple analytic expression for the evolution of the feedback parameter λt), the radiation fluxes, and the resulting increase in OHC.

From these PEMs we can easily compare the global performance of different ESMs under different forcing scenarios. For instance, a comparison of the GISS-E2-R and CESM104 models exhibit equilibrium climate sensitivities (ECSs) of 3.4  and 2.4 K, respectively. The main reason for the difference is very different albedo feedbacks in the two models. Resulting total feedback parameter  λ(t) drops from 2.1 to 1.0 Wm-2 K-1 in GISS-E2-R and from 1.4 to 0.6 Wm-2 K-1 in CESM104. The OHC grows at nearly the same rate in the two models during the first millenium, but GISS saturates earlier and at lower final OHC.

How to cite: Rypdal, K.: Parsimonious models emulating millennium-long Earth system model simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12585, https://doi.org/10.5194/egusphere-egu26-12585, 2026.

EGU26-12666 | Orals | NP1.2

Exploring state dependence of the climate response to radiative forcing using two idealized coupled climate models 

Christopher Pitt Wolfe, Youwei Ma, Anna Katavouta, Kevin Reed, and Richard Williams

Studies of climate sensitivity and feedbacks typically employ a suite of models with similar base climates but different model physics. Such an approach is useful for uncovering how changes to physical processes affect the climate response to changes in radiative forcing, but obscures the dependence of the climate response on the initial state of the climate itself. In order to better understand this dependence, we study the response to radiative forcing of two nearly identical configurations of the Community Earth System Model (CESM) with production-grade physics and resolutions that have dramatically different climates. The first, called Aqua, is completely covered with a uniform-depth ocean except for two 10º-wide polar continents to avoid the polar singularities in the ocean model. The second, Ridge, is identical to Aqua except for the presence of a thin ridge continent connecting the two polar caps. The ridge supports gyres in the ocean and leads to a warm, ice-free climate resembling a global Pacific Ocean, with a warm pool and cold tongue in the tropical ocean connected by a Walker circulation in the atmosphere. In contrast, the mean climate of Aqua is zonally symmetric and dominated by a global cold belt in the ocean driven by vigorous equatorial upwelling. The lack of gyres leads to a deep oceanic thermocline and reduces meridional heat transport, which allows for the development of persistent sea ice at high latitudes.

These two mean climates are perturbed by increasing atmospheric CO2 concentration at a rate of 1% per year until quadrupling. Aqua initially warms more slowly than Ridge, with the transient climate response (TCR) at doubling 23% smaller for Aqua than Ridge. After doubling, however, Aqua begins to warm faster than Ridge and Aqua’s global mean temperature surpasses Ridge’s at quadrupling. A linear feedback analysis is used to gain insight into the time-evolving responses of these two configurations to increased CO2 concentration. At all stages, Aqua’s net top-of-the-atmosphere heating is greater than Ridge’s. At early times, this is due to high clouds replacing low clouds in Aqua’s high latitudes, but decreasing surface albedo due to sea-ice loss eventually becomes a dominant factor. Aqua’s deep thermocline supports a higher ocean heat uptake (OHU) efficiency relative to Ridge that initially offsets these positive feedbacks and results in Aqua’s lower TCR. As CO2 concentration approaches quadrupling, the combined effects of declining OHU efficiency and a strengthening ice-albedo feedback drive Aqua’s warming to temperatures compatible to Ridge. In the century following quadrupling, Aqua warms several Kelvin more than Ridge.

These idealized systems can shed light on the fundamental aspects of Earth’s climate system—such as how the response to radiative forcing depends on the base climate—that might be obscured in more complex configurations.



How to cite: Pitt Wolfe, C., Ma, Y., Katavouta, A., Reed, K., and Williams, R.: Exploring state dependence of the climate response to radiative forcing using two idealized coupled climate models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12666, https://doi.org/10.5194/egusphere-egu26-12666, 2026.

EGU26-13950 | Orals | NP1.2 | Highlight

Understanding regional discrepancies using the climate model hierarchy 

Tiffany Shaw and Joonsuk Kang

As Earth warms, regional climate signals are accumulating. Some signals, for example, land warming more than the ocean and the Arctic warming the most, were expected and successfully predicted. Underlying this success was the application of physical laws across a climate model hierarchy under the assumption that large and small spatial scales are well separated. With additional warming, however, discrepancies between real-world signals and model predictions are accumulating, especially at regional scales. In this talk, we will highlight the emerging list of model-observation discrepancies in historical trends. We demonstrate how the climate model hierarchy can be used to understand the physical processes underlying these discrepancies. We argue that progress can be made by filling gaps in the hierarchy and making more process-informed observations.

How to cite: Shaw, T. and Kang, J.: Understanding regional discrepancies using the climate model hierarchy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13950, https://doi.org/10.5194/egusphere-egu26-13950, 2026.

EGU26-14266 | ECS | Orals | NP1.2

Rate-dependent Tipping of the AMOC under CO2 increase in an Intermediate Complexity Model 

Sjoerd Terpstra, Swinda Falkena, Robbin Bastiaansen, and Anna von der Heydt

The stability of the Atlantic Meridional Overturning Circulation (AMOC) under future climate change remains uncertain. While most climate models across the model hierarchy project a weakening or collapse under freshwater forcing, transient simulations under increasing CO2 levels also commonly show a weakening or even a collapse of the AMOC. However, longer equilibrium experiments---primarily conducted with lower-complexity models due to computational costs---show more varied responses to CO2 forcing. While most models show an initial weakening of the AMOC, some models equilibrate to a weak AMOC state only at very high CO2 levels, while others equilibrate to a stronger-than-present AMOC. One such model is the intermediate complexity model CLIMBER-X, which (in equilibrium) shows that the AMOC strengthens until at least 16 times preindustrial CO2 levels are reached. However, during the transient phase of increasing CO2, the AMOC weakens. This suggests that the AMOC's transient response may differ from its equilibrium behavior. This raises the question: can the AMOC collapse under rapid and high CO2 increase, even if a stable equilibrium state exists? 

We show that the AMOC exhibits rate-dependent tipping; when CO2 increases fast enough and reaches sufficiently high levels, the AMOC can fully collapse. This occurs under very high forcing, starting from 7 times preindustrial CO2 levels and a rate of 2.0% ppm/yr CO2 increase. This collapse occurs despite the existence of a stable AMOC at equilibrium. By examining the physical processes through which the collapse occurs, we contribute to the understanding of the AMOC response in a warming climate. By also incorporating freshwater forcing, we assess the risks of rapid warming on the AMOC stability. Our results show that even models with a stable equilibrium AMOC under high CO2 levels can experience weakening during the transient phase or even collapse. This highlights the need to assess both the rate and magnitude of CO2 forcing when assessing the stability of the AMOC. While this effect occurs at very high CO2 levels in CLIMBER-X, the role of the rate of CO2 increase may become relevant at lower CO2 levels when combined with freshwater forcing. Our findings demonstrate that the AMOC can undergo rate-dependent tipping under rapid and high CO2increase, even if a stable AMOC exists at very high CO2 levels.

How to cite: Terpstra, S., Falkena, S., Bastiaansen, R., and von der Heydt, A.: Rate-dependent Tipping of the AMOC under CO2 increase in an Intermediate Complexity Model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14266, https://doi.org/10.5194/egusphere-egu26-14266, 2026.

EGU26-14741 | Posters on site | NP1.2

Coupled ESM-IAM Emulator: Exploring Uncertainties in Temperature Target Pathways 

Katsumasa Tanaka, Xiong Weiwei, Myles Allen, Michelle Cain, Stuart Jenkins, Camilla Mathison, Vikas Patel, Chris Smith, and Kaoru Tachiiri

Integrating physical, socio-economic, and technological perspectives is indispensable for addressing climate mitigation challenges. While directly coupling state-of-the-art Earth System Models (ESMs) and Integrated Assessment Models (IAMs) offers a way to explore feedbacks between these domains, doing so with full-complexity models remains computationally prohibitive. This is particularly true for cost-effective intertemporal optimization IAMs due to fundamental operational differences: while ESMs perform forward simulations, such IAMs optimize over time. Consequently, direct coupling would require numerous computationally intensive iterations to converge, a complication further compounded by the stochastic nature of ESMs.

To overcome the barriers to coupling ESMs and IAMs, we employ their reduced-complexity representations (i.e., emulators). We couple an IAM emulator representing 9 distinct IAMs (Xiong et al. 2025) with an ESM emulator, FaIR, representing 66 ESM configurations (Smith et al. 2024a). Using this coupled ESM-IAM emulator framework in an optimization setting, we calculate cost-effective pathways that achieve the temperature targets of the Paris Agreement with and without overshoot.

Our preliminary results indicate that the uncertainty ranges for such pathways are significantly larger than previously estimated. Our results also have implications for target setting; we show how pathways differ when IAMs optimize directly for a temperature target – a capability IAMs traditionally lack. Instead, IAMs typically rely on temperature proxies, such as carbon budgets (or their corresponding carbon price pathways), which do not necessarily provide an accurate representation of the temperature target. Furthermore, this study offers advanced insights into the dynamics of climate-economy interactions, providing a roadmap for future efforts to couple full-complexity models.

 

References

Xiong, W., Tanaka, K., Ciais, P., Johansson, D. J. A., & Lehtveer, M. (2025). emIAM v1.0: an emulator for integrated assessment models using marginal abatement cost curves. Geosci. Model Dev., 18(5), 1575-1612. doi:10.5194/gmd-18-1575-2025

Smith, C., Cummins, D. P., Fredriksen, H. B., Nicholls, Z., Meinshausen, M., Allen, M., . . . Partanen, A. I. (2024). fair-calibrate v1.4.1: calibration, constraining, and validation of the FaIR simple climate model for reliable future climate projections. Geosci. Model Dev., 17(23), 8569-8592. doi:10.5194/gmd-17-8569-2024

How to cite: Tanaka, K., Weiwei, X., Allen, M., Cain, M., Jenkins, S., Mathison, C., Patel, V., Smith, C., and Tachiiri, K.: Coupled ESM-IAM Emulator: Exploring Uncertainties in Temperature Target Pathways, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14741, https://doi.org/10.5194/egusphere-egu26-14741, 2026.

EGU26-15472 | ECS | Posters on site | NP1.2

Low Uncertainty Regional Climate Projections without Irrelevant Weather Details 

Yifan Wang, Shaun Lovejoy, Dustin Lebiadowski, and Dave Clarke

Uncertainties in conventional (GCM) climate models, defined as the structural spread among com-
peting models, have increased for the first time in the latest AR6 report despite an exponential increase
in the modern computation power. The root problem is that these models are based in the weather
regime, that is, they spend unnecessary effort in calculating irrelevant weather details. This project
aims to produce precise regional projection using the Half Order Energy Balance Equation (HEBE): a
half order fractional derivative generalization of the standard Energy Balance Equation (EBE). HEBE
has the advantage of being a direct consequence of the continuum heat equation combined with energy-
conserving surface boundary conditions. A previous paper used Fractional EBE (FEBE) to model Earth
climate projections through 2100 on a global scale, and it yields significantly smaller uncertainty com-
pared to the CMIP6 MME. This project builds on a similar methodology, enhancing climate projection
with additional regional details and upgraded precision. The current results show that the parametric
uncertainty in HEBE’s temperature response is smaller than the internal variability at most locations,
at the exceptions of the high memory deep ocean regions near Pacific. HEBE’s regional hindcast ac-
curately reproduces ERA5 2mT series’ deterministic and stochastic patterns of regional temperature.
The global hindcast is also validated by various reanalysis datasets and instrumental records. The
direct year to year relative uncertainty (ratio between 90% confidence interval and best estimate) is
stable across time and marker scenarios, with most regions projecting values below 0.5 by 2100. On a
global scale, the parametric uncertainty in HEBE’s response temperature is negligible (±0.03K by 2100
using the SSP2-4.5 marker scenario). This effectively shows that HEBE’s projection is more precise
than its competitors even without taking period averages. The exceedingly low global uncertainty was
constrained by the large amount of regional information when taking the global averages. It should be
noted that the cited parametric uncertainty does not take into account systematic biases in HEBE and
in the input datasets. The most important source should be any errors in the forcings, especially con-
cerning aerosols. HEBE aims to provide a compelling and physically grounded alternative to complex
deterministic multi-model ensembles, offering a more precise, efficient, and interpretable means of pro-
jecting regional climate changes in the coming century. This positions it as a potentially valuable tool
for policy-relevant projections and adaptation planning, thereby showing the pertinency of fractional
derivative and Bayesian framework in atmospheric sciences.

How to cite: Wang, Y., Lovejoy, S., Lebiadowski, D., and Clarke, D.: Low Uncertainty Regional Climate Projections without Irrelevant Weather Details, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15472, https://doi.org/10.5194/egusphere-egu26-15472, 2026.

EGU26-16369 | Posters on site | NP1.2

The future is in the past? A flexible resampling approach to generate multivariate time series 

Michael Lehning, Tatjana Milojevic, and Pauline Rivoire

Synthetic time series generation is an essential tool for robustly exploring different climate scenarios and their impacts. While sophisticated generation methods have been developed in the past, they often rely on physical and statistical assumptions and require extensive data for calibration and parameter estimation. We propose a straightforward method for time series generation based on constrained sampling of observations. This approach preserves the physical consistency between variables and maintains the short temporal structure present in the observation. We apply this procedure to generate temperature, precipitation, incoming solar radiation, and wind speed time series sampled from meteorological station observations. We obtain different sets of synthetic time series by constraining the mean temperature according to future scenarios provided by climate model projections. We show that the sampled time series preserve the multivariate dependence structure observed in both historical data and climate projections. While, by design, the method does not generate daily values beyond the observed range, it can simulate multi-day extremes that exceed those in the observational record, such as longer heatwaves. The approach is flexible and can be applied to other variables with other constraints, provided that a sufficiently long observational time series is available and the constraints are compatible with the observed data. The generation procedure may thus prove useful for studying potential future extremes and help in general downscaling tasks.

How to cite: Lehning, M., Milojevic, T., and Rivoire, P.: The future is in the past? A flexible resampling approach to generate multivariate time series, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16369, https://doi.org/10.5194/egusphere-egu26-16369, 2026.

Reservoirs are increasingly recognized as significant sources of greenhouse gas (GHG) emissions, yet their future emissions under climate change remain poorly quantified. This study evaluates the impact of climate change on net GHG emissions from Feitsui Reservoir, a major water supply reservoir in northern Taiwan, using an integrated modeling approach.

We utilized the multisite Weather Generator (multiWG) to generate future climate projections for three Shared Socioeconomic Pathways (SSP126, SSP245, SSP585) across four 20-year periods (2021-2040, 2041-2060, 2061-2080, 2081-2100), with 1995-2014 as the baseline. A Random Forest model (NSE = 0.8637) was trained to predict reservoir inflow based on temperature and precipitation data. These inflows were input into the G-RES model to calculate net GHG emissions in CO₂-equivalent units, including contributions from both CO₂ and CH₄.

Results reveal that reservoir GHG emissions will increase under all climate scenarios, with magnitude strongly dependent on emission pathways. Under the low-emission scenario (SSP126), emissions increase by 5.2-8.8% across all periods. The intermediate scenario (SSP245) shows moderate increases of 5.4-18.4%. The high-emission scenario (SSP585) demonstrates dramatic escalation, particularly in the late century (2081-2100), where emissions reach 1259.6 gCO₂e/m²/yr—a 45.8% increase. These findings underscore the critical need to consider climate impacts in reservoir management and carbon accounting frameworks.

How to cite: Yeh, F.-W. and Tung, C.-P.: Assessing Climate-Driven Greenhouse Gas Emissions from Feitsui Reservoir Using G-RES Under Multiple SSP Scenarios, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16498, https://doi.org/10.5194/egusphere-egu26-16498, 2026.

EGU26-16683 | Orals | NP1.2

Combining emulators and demographics: Building a flexible toolkit for lifetime exposure assessments 

Quentin Lejeune, Rosa Pietroiusti, Amaury Laridon, Niklas Schwind, Carl-Friedrich Schleussner, and Wim Thiery

Across the globe, today’s young generations will be more frequently exposed to climate extremes over their lifetime than earlier generations. Previous work has established this finding by combining simulations of historical and projected trends in climate extremes together with data on past and future demographic changes (Thiery et al. 2021, Grant et al. 2025). However, it has so far focused on a limited set of climate extreme indicators, using climate (impact) simulations from ISIMIP2 and demographics datasets that are now outdated, and did not fully assess uncertainty across the climate impact modelling chain. 

 

We now build on this existing lifetime exposure framework and combine it with a chain of emulators constituted of a Simple Climate Model (SCM) and the Rapid Impact Model Emulator Extended (RIME-X, Schwind et al., submitted). RIME-X can translate the GMT distributions generated by an SCM for a given emission scenario into spatially explicit distributions of climate or climate impact indicators. It has already been used to produce projections for 40+ indicators derived from ISIMIP3 and other climate model simulations, and this list can be extended to further indicators whose evolution predominantly depends on the level of global warming and for which historical and future simulations are available.   

 

We also update the lifetime exposure framework to consider more recent demographic data, and package it into a GitHub repository called dem4cli (short for ‘demographics for climate’) that will be made publicly available. We use spatially explicit population reconstructions and projections from the COMPASS project, and national-level life expectancy and cohort size estimates and projections from UNWPP2024.  

 

This work delivers more robust calculations of lifetime exposure to changes in extremes or climate impacts, by leveraging the ability of the SCM-RIME-X emulator chain to represent both their forced response to emissions as well as the combined uncertainty arising from the GMT response to emissions, the local climate response to global warming, and interannual variability, in combination with updated demographic data. This new framework is designed to generate such policy-relevant information in a more flexible and systematic manner, as it can in theory be applied to any available emission or GMT trajectories, and extended to a broad range of climate hazards.

Thiery, W. et al. Intergenerational inequities in exposure to climate extremes. Science 374, 158–160 (2021) 

Grant, L., Vanderkelen, I., Gudmundsson, L. et al. Global emergence of unprecedented lifetime exposure to climate extremes. Nature 641, 374–379 (2025) 

Schwind et al. RIME-X v1.0: Combining Simple Climate Models, Earth System Models, and Climate Impact Models into a Unified Statistical Emulator for Regional Climate Indicators. Geoscientific Model Development (submitted) 

How to cite: Lejeune, Q., Pietroiusti, R., Laridon, A., Schwind, N., Schleussner, C.-F., and Thiery, W.: Combining emulators and demographics: Building a flexible toolkit for lifetime exposure assessments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16683, https://doi.org/10.5194/egusphere-egu26-16683, 2026.

EGU26-16747 | ECS | Orals | NP1.2

The effect of freshwater biases on AMOC stability across the model complexity spectrum 

Amber Boot and Henk Dijkstra

A collapse of the Atlantic Meridional Overturning Circulation (AMOC) would have strong consequences for the global climate system.  Assessing whether the AMOC will collapse in the future is difficult since current Earth System Models (ESMs) have biases. An earlier study using an intermediate complexity Earth system model (EMIC) showed the potential effect of freshwater biases on AMOC stability.  However, the used model has a limited ocean model with respect to the used  resolution and processes represented compared to ESMs. Here, we supplement the EMIC simulations with simulations of an ocean-only model using the same resolution as is typically used in ESMs. This allows us to study the effect of ocean resolution on the physical mechanism controlling the effect of freshwater biases on AMOC stability. We find that both the intermediate complexity and the ocean-only model behave qualitatively similar. In both models freshwater biases influence AMOC stability where negative (positive) biases in the Indian Ocean tend to stabilize (destabilize) the AMOC, whereas the opposite applies to biases in the Atlantic Ocean. Based on the freshwater biases present in most ESMs, our results suggest that most ESMs have a too stable AMOC and might therefore underestimate the probability of an AMOC collapse under future emission scenarios.

How to cite: Boot, A. and Dijkstra, H.: The effect of freshwater biases on AMOC stability across the model complexity spectrum, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16747, https://doi.org/10.5194/egusphere-egu26-16747, 2026.

EGU26-17291 | ECS | Posters on site | NP1.2

Using Ice Cores and Gaussian Process Emulation to Recover Changes in the Greenland Ice Sheet During the Holocene 

Irene Malmierca Vallet, Louise C. Sime, Jochen Voss, Diego Fasoli, and Kelly Hogan

The shape and extent of the Greenland Ice Sheet (GIS) during the Holocene remain a matter of considerable debate, with existing studies proposing a wide range of reconstructions. In this study, we aim to combine stable water isotopic information from ice cores with outputs from isotope-enabled climate models to investigate this problem. Directly exploring the space of possible ice sheet geometries through numerical simulations is computationally prohibitive. To address this challenge, we plan to develop a Gaussian process emulator that will serve as a statistical surrogate for the full climate model. The emulator will be trained on the results of a limited number of carefully designed simulations and will be used to enable fast, probabilistic predictions of model outputs at untried inputs. The inputs will consist of GIS morphologies, parameterized using a dimension-reduction technique adapted to the spherical geometry of the ice sheet. Using predictions from the emulator, we will explore the range of ice sheet morphologies that are compatible with available ice-core isotope measurements and other complementary observational data, including those collected during recent KANG-GLAC expeditions, with the goal of ultimately reducing uncertainty in reconstructions of Holocene GIS morphology.

How to cite: Malmierca Vallet, I., Sime, L. C., Voss, J., Fasoli, D., and Hogan, K.: Using Ice Cores and Gaussian Process Emulation to Recover Changes in the Greenland Ice Sheet During the Holocene, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17291, https://doi.org/10.5194/egusphere-egu26-17291, 2026.

EGU26-18639 | Posters on site | NP1.2

The compact Earth system model OSCAR v4 

Thomas Gasser, Biqing Zhu, Xinrui Liu, Danni Zhang, Yuqin Lai, and Gaurav Shrivastav

OSCAR is an open-source reduced-complexity Earth system model designed to probabilistically emulate the coupled climate–carbon–chemistry system with low computational cost. Following a preivously published evaluation of OSCAR v3.1 against observations and CMIP6 Earth system models, we present OSCAR v4, which incorporates a range of structural, numerical, and methodological improvements. Key developments include enhanced numerical stability, modularization of the code to allow running submodels independently, revised and streamlined modules, and recalibration using the latest AR6, CMIP6, and TRENDY datasets. Monte Carlo sampling has been improved using continuous probability distributions, and the constraining strategy now leverages Latin-hypercube sampling combined with probability integral transforms to provide more robust probabilistic ensembles compatible with observations. Alongside core model improvements, OSCAR v4 will introduce a suite of user-oriented functionalities and a full online documentation, facilitating broader adoption and reproducibility.

We illustrate the performance of OSCAR v4 through participation in the Reduced Complexity Model Intercomparison Project (RCMIP) phase 3 exercise. This benchmarking demonstrates the model’s ability to reproduce the spread of global temperature and carbon-cycle responses observed in more complex Earth system models, while providing rapid, policy-relevant probabilistic projections. Given it's level of complexity, OSCAR v4 is positioned as a versatile tool bridging comprehensive Earth system models and the simpler reduced-complexity approaches for large-scale climate assessments.

How to cite: Gasser, T., Zhu, B., Liu, X., Zhang, D., Lai, Y., and Shrivastav, G.: The compact Earth system model OSCAR v4, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18639, https://doi.org/10.5194/egusphere-egu26-18639, 2026.

EGU26-19277 | Orals | NP1.2

From scenarios to impacts – an emulation of regional climate impacts and their uncertainties using the CMIP7 mitigation scenarios    

Daniel Hooke, Camilla Mathison, Eleanor Burke, Chris Jones, Laila Gohar, and Andy Wiltshire

The PRIME (Mathison et al. 2025) framework provides a fast response tool to look at climate impacts for up-to-date mitigation scenarios. PRIME combines the FaIR simple climate model and pattern scaling of Earth System Models (ESMs) with the JULES land surface model to quantify spatially resolved climate impacts. In addition, PRIME samples uncertainty from both the spatial patterns of CMIP6 ESMs and the probabilistic configuration of the latest version of FaIR. 

We present applications of this framework to explore impacts on both the earth system and potential impacts on societies, using new scenarios produced for CMIP7. From an earth system perspective, we use an updated configuration of JULES incorporating permafrost processes and fire to look at the impact of the northern high latitude net ecosystem balance. In terms of societal impacts, we simulate the potential impacts of climate change on agricultural drought of rain fed crops during the growing season. This analysis includes a quantification of the uncertainty derived from the global mean climate response and the spatial responses of ESMs. Results from PRIME will also be part of the FastMIP project. 

How to cite: Hooke, D., Mathison, C., Burke, E., Jones, C., Gohar, L., and Wiltshire, A.: From scenarios to impacts – an emulation of regional climate impacts and their uncertainties using the CMIP7 mitigation scenarios   , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19277, https://doi.org/10.5194/egusphere-egu26-19277, 2026.

EGU26-19612 | ECS | Posters on site | NP1.2

Accounting for Aerosols in Climate Mitigation Pathways 

Tomás Arzola Röber, Thomas Bruckner, and Johannes Quaas

To meet Paris-aligned climate goals and minimize temperature overshoot and its impacts, rapid and deep reductions in greenhouse-gas emissions from fossil-fuel combustion are required. Climate risk projections are strongly affected by uncertainty in anthropogenic aerosol effective radiative forcing (ERF) and by the co-evolution of air-pollutant emissions under decarbonization pathways. Because running large Earth System Model (ESM) ensembles remains computationally expensive for uncertainty quantification and broad policy-scenario exploration, reduced-complexity climate emulators are needed for efficient, transparent, and observation-connected assessments.

Here we develop an aerosol extension to the simple climate model (SCM) FaIR that emulates aerosol ERF from global anomalies in aerosol optical depth (ΔAOD) relative to a pre-industrial baseline for different species. Aerosol ERF is computed using a constrained parameterization that separates aerosol–radiation and aerosol–cloud interactions, with key parameters represented probabilistically and constrained by observational and model-based lines of evidence.

To emulate ΔAOD from emissions pathways, we implement an interpretable mapping calibrated to CMIP6 ESM output. An effective linear relationship between emission and burden anomalies is fitted using a single parameter that aggregates yield and lifetime effects. In a second step, we fit an effective optical parameter linking burden perturbations to ΔAOD. This produces model-dependent parameter distributions that enable propagation of both parametric uncertainty and between-model spread. In addition, we implement an integrated-assessment-model-based relationship linking air-pollutant emissions to CO₂ emissions under different air-quality policy stringencies, interpolated into a continuous air-quality parameter suitable for exploring uncertainty and its interaction with decarbonization trajectories.

We perform Monte Carlo ensembles sampling aerosol-ERF parameters, CMIP6-calibrated aerosol–AOD mappings, air-quality policy stringency, and net-zero timing, and evaluate impact-relevant climate risk metrics including peak warming, probability of remaining below 1.5 °C, threshold crossing year, overshoot duration, and warming rates computed over multiple near-term and decadal windows. Preliminary results show strong dependence of peak temperature outcomes on net-zero timing, while threshold-based metrics and warming rates exhibit pronounced sensitivity to air-quality assumptions, consistent with a partial loss of aerosol cooling under stricter pollution controls. Overall, the results indicate non-linear interactions between decarbonization timing, air-quality stringency, and warming-rate responses. The emulator provides a scalable basis for robust climate risk screening and for coupling SCM trajectories to impact assessments.

Keywords: Climate Change, Mitigation, Aerosols, Effective Radiative Forcing, Climate Emulators, Climate Modeling, CMIP6 Calibration, Air-quality Policy, Overshoot

How to cite: Arzola Röber, T., Bruckner, T., and Quaas, J.: Accounting for Aerosols in Climate Mitigation Pathways, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19612, https://doi.org/10.5194/egusphere-egu26-19612, 2026.

EGU26-20117 | Posters on site | NP1.2

Applying GWP* to Long-Term Climate Pathways and Fluorinated Gases 

Michelle Cain, Vikas Patel, Matteo Mastropierro, Katsumasa Tanaka, Stuart Jenkins, and Myles Allen

Greenhouse gas emission metrics are widely used for comparing climate impacts of different gases and for guiding mitigation policy. Conventional metrics such as GWP100 perform well for representing the warming effects of long-lived gases which behave like CO₂ but poorly for short-lived climate pollutants (SLCPs). Methane (CH4) is the most important SLCP and has been the main focus of alternative metrics. GWP* was developed to more accurately capture impact on global warming, particularly from stable and declining CH4 emissions which are not well served by GWP100. This means that GWP* better connects emissions pathways to long-term temperature targets (Cain et al., 2022). Previous studies optimised GWP* for CH4 for a limited range of scenarios up to 2100. However, future mitigation pathways involve a wider range of gases and transition speeds, overshoot behaviour, and long-term stabilization beyond this period. In addition, highly radiatively efficient fluorinated gases are increasingly important in mitigation strategies yet have not been demonstrated with the GWP* framework. In this study, we systematically test the performance of GWP* across an expanded set of emissions scenarios, including rapid mitigation, delayed action, and prolonged temperature overshoot pathways, and extend the analysis to multi-century time horizons with an optimisation of the flow term of GWP* (Mastropierro et al., 2025). We further develop and evaluate a generalized formulation of GWP* for fluorinated gases with diverse atmospheric lifetimes. The outcomes examine the performance of GWP* under realistic transition pathways and its representation of temperature responses for fluorinated gases. This work supports the development of more physically consistent multi-gas emission metrics for climate targets, carbon budgeting, and policy design, as it is a simple tool to calculate how much global warming is added or avoided by increasing or cutting SLCPs such as F-gases.

Cain, M., Jenkins, S., Allen, M.R., Lynch, J., Frame, D.J., Macey, A.H., Peters, G.P. Methane and the Paris Agreement temperature goals. Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 380 (2022). https://doi.org/10.1098/rsta.2020.0456

Mastropierro, M., Tanaka, K., Melnikova, I. et al. Testing GWP* to quantify non-CO2contributions in the carbon budget framework in overshoot scenarios. npj Clim Atmos Sci 8, 101 (2025). https://doi.org/10.1038/s41612-025-00980-7

How to cite: Cain, M., Patel, V., Mastropierro, M., Tanaka, K., Jenkins, S., and Allen, M.: Applying GWP* to Long-Term Climate Pathways and Fluorinated Gases, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20117, https://doi.org/10.5194/egusphere-egu26-20117, 2026.

EGU26-20145 | Posters on site | NP1.2

Investigating the possibility of rare spontaneous AMOC transitions in the intermediate complexity climate model FAMOUS. 

Jeroen Wouters, Guannan Hu, Jochen Bröcker, and Robin Smith

Earth System Models of Intermediate Complexity (EMICs) allow for fast exploration of large-scale climate dynamics. These models thus enable the development and testing of large-ensemble-based techniques that would be too costly with more realistic climate models.

In this ongoing study we develop a rare event simulation setup to explore the possibility of a spontaneous collapse of the Atlantic Meridional Overturning Circulation (AMOC) in the FAMOUS model. FAMOUS is a low-resolution, coupled atmosphere-ocean general circulation model derived from the UK Met Office’s Unified Model specifically designed for efficient, long-duration and ensemble climate simulations. FAMOUS has previously been used to investigate the hysteresis of the Atlantic Meridional Overturning Circulation under freshwater hosing.

We apply a genealogical particle analysis (GPA) algorithm that is designed to probe the possibility of spontaneous AMOC transitions. The method initiates an ensemble of realisations in the "on"-state of the AMOC and clones ensemble members at regular intervals  that are showing a low AMOC.

Contrary to recent results in another EMIC, a straightforward sampling based on the AMOC indicator does not result in any spontaneous transitions to the AMOC "off"-state. To improve the selection of potentially exceedingly rare trajectories, we therefore investigate statistical methods to identify physical variables that correlate with the state of the AMOC ahead of time, to be used as selection criteria in the GPA algorithm.

How to cite: Wouters, J., Hu, G., Bröcker, J., and Smith, R.: Investigating the possibility of rare spontaneous AMOC transitions in the intermediate complexity climate model FAMOUS., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20145, https://doi.org/10.5194/egusphere-egu26-20145, 2026.

EGU26-20975 | ECS | Posters on site | NP1.2

Modelling Mesoarchaean climate: Economic implications  

Lisa Wasitschek, Hartwig E. Frimmel, Nina Hiby, and Felix Pollinger

The Witwatersrand Basin on the Kaapvaal Craton hosts the world’s largest gold province, with the vast majority of gold concentrated in the 2.90–2.79 Ga Central Rand Group, whereas the slightly older 2.95–2.91 Ga West Rand Group is largely barren despite comparable sedimentary characteristics. This contrast has been attributed to intensified chemical weathering during Central Rand Group times, which promoted enhanced gold mobilisation from the Archaean hinterland. However, the climatic and environmental drivers of this weathering intensification remain poorly constrained. To address this, we investigated Mesoarchaean climate controls using the Planet Simulator (PlaSim), an Earth system model of intermediate complexity. We conducted 140 PlaSim simulations to quantify the climatic sensitivity to atmospheric greenhouse gas concentrations, continental surface area, surface albedo, and land configuration. CO₂-equivalent concentrations (3–30 %), land coverage (8–28 %), and albedo (0.15–0.30) were systematically varied across different land distributions (equatorial, polar and spread over different latitudes).

Next to the well-known effect of global warming under increased greenhouse gas concentrations, our results show that increasing continental area generally results in global cooling due to the higher albedo of land surfaces relative to oceans, particularly when land was concentrated at low latitudes. This cooling effect becomes pronounced once land exceeds approximately 13 % of Earth’s surface. At high latitudes, land has minimal climatic impact because of the low incoming radiation angle that leads to less absorption. Exceptions are noted under conditions of low greenhouse gas concentrations and low surface albedo, at which limited land growth could slightly enhance warming. Among the tested land positions, the scenario with land spread over different latitudes resulted in the highest climate sensitivity.

Overall, our results indicate that land distribution alone was unlikely to have caused global warming during the Mesoarchaean, and this climatic influence was probably dampened by a more rapid carbon cycle at that time. Instead, elevated atmospheric greenhouse gas levels emerge as the dominant driver of warming and enhanced chemical weathering. The climatic transition around ~2.9 Ga may further reflect the emergence of extensive low-albedo mafic or ultramafic surfaces and/or the latitudinal migration of the Kaapvaal Craton into a more radiatively sensitive, low-latitude zone. These combined factors likely contributed to intensified weathering, increased gold leaching, and the gold megaevent responsible for the formation of the Witwatersrand ores.

How to cite: Wasitschek, L., Frimmel, H. E., Hiby, N., and Pollinger, F.: Modelling Mesoarchaean climate: Economic implications , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20975, https://doi.org/10.5194/egusphere-egu26-20975, 2026.

EGU26-21556 | ECS | Posters on site | NP1.2

Surface albedo as a first-order control on Mesoarchaean climate (PlaSim) 

Nina Hiby, Lisa Wasitschek, and Hartwig E. Frimmel

The radiative balance of the early Earth was governed by other boundary conditions than today, including a fainter Sun, elevated greenhouse gas concentrations, and a smaller land surface area. Although the role of atmospheric composition in sustaining habitable surface temperatures during the Mesoarchaean has been extensively investigated, especially to solve the faint young Sun paradox, the climatic impact of land position and distribution under varying albedo remains comparatively underexplored.

We therefore assess how variations in land-surface albedo, land fraction, and land distribution could have modulated Mesoarchaean climate states. Using the Planet Simulator (PlaSim), an intermediate-complexity climate model, we conducted 195 simulations spanning CO₂-equivalent forcing levels of 3–10 % (30,000–100,000 ppm). Land-surface albedo was varied between 0.15 and 0.30, land area between 8 % and 28 %, and idealised land distributions were prescribed, including diagonal, staggered, and mid-latitude configurations. Ocean albedo was held constant at 0.144 to isolate the climatic impact of continental reflectivity.

Across all simulations, global mean temperature responds strongly and non-linearly to both land fraction and land albedo. At low land albedo (0.15) and low to intermediate CO₂-equivalent forcing (3–5 %), increasing land area produces a slight warming trend, despite minimal differences between land and ocean reflectivity. This behaviour indicates that land–ocean contrasts in surface energy partitioning and effective heat capacity can modify global climate even when shortwave albedo contrasts are small. Sensitivity increases abruptly as land albedo rises from 0.20 to 0.25. Beyond this threshold, modest increases in land area result in pronounced global cooling, consistent with a regime shift in the radiative balance. This non-linear response is most prominent at low to intermediate CO₂-equivalent forcing and becomes progressively muted at higher forcing (10 %), where greenhouse effects dampen the temperature response to surface reflectivity changes. The pattern occurs across all land configurations but is amplified when landmasses occupy equatorial to mid-latitudes, where insolation is highest and albedo exerts maximum leverage, whereas high-latitude land has a comparatively weaker effect.

These findings highlight that land surface characteristics such as albedo and distribution were critical for early Earth’s climate. Even under strongly greenhouse-forced atmospheres, surface properties significantly altered the planetary energy budget. Recognising such sensitivities is essential for reconstructing Archaean climate states and assessing the potential for climatic stability under reduced solar luminosity.

How to cite: Hiby, N., Wasitschek, L., and Frimmel, H. E.: Surface albedo as a first-order control on Mesoarchaean climate (PlaSim), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21556, https://doi.org/10.5194/egusphere-egu26-21556, 2026.

EGU26-21970 | ECS | Posters on site | NP1.2

Simulating NAO-driven AMOC collapse in the PlaSim-LSG Climate Model 

Arianna Magagna, Giuseppe Zappa, Matteo Cini, and Susanna Corti

The Atlantic Meridional Overturning Circulation (AMOC) is a critical component of the global climate system and its potential for abrupt collapse represents a significant tipping point. Our project investigates whether a persistent negative phase of the North Atlantic Oscillation (NAO), a dominant mode of atmospheric variability, can induce an AMOC collapse in the absence of external perturbations within the coupled PlaSim-LSG climate model of intermediate complexity. A control simulation establishes a baseline climatology, confirming that NAO variability leads AMOC fluctuations by approximately one year. To overcome the computational limitation of simulating rare events, we implement a rare event algorithm (GKLT) that efficiently biases the model toward trajectories with negative NAO conditions over 125-year simulations. The results reveal a fundamental bistability in the system. While persistent negative NAO forcing can trigger an AMOC collapse, the outcome is probabilistic: out of six independent ensemble simulations, four evolved entirely into a collapsed state (∼ 12 Sv), one remained entirely vigorous (∼ 23 Sv) and one split into both outcomes. A cluster-based analysis traces this divergence to the early amplification of small differences in North Atlantic heat fluxes, convection and sea-ice cover. These findings show that internal atmospheric variability alone can force the AMOC across a tipping point, highlighting the role of internal climate dynamics in shaping climate transitions.

How to cite: Magagna, A., Zappa, G., Cini, M., and Corti, S.: Simulating NAO-driven AMOC collapse in the PlaSim-LSG Climate Model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21970, https://doi.org/10.5194/egusphere-egu26-21970, 2026.

On 3 May 2025, a severe hailstorm affected Paris and parts of western Europe. We assess whether anthropogenic climate change contributed to its intensity using ERA5 reanalyses and an analogue-based attribution framework. The synoptic pattern featured a cut-off low and a surface cold front following several warmer-than-normal days. We identify circulation analogues to 3 May 2025 in two periods, namely a cooler “past” (1974–1999) and a warmer “present” (1999–2024). We then compare thermodynamic conditions under otherwise similar large-scale flow. Hail probability and size are estimated with two models: (i) a logistic formulation using Convective Available Potential Energy (CAPE), deep-layer wind shear, and convective precipitation, and (ii) an extended model including freezing-level height and 850 hPa temperature, tailored to European hail environments. Models are calibrated with ˆIle-de-France observations and validated independently. Present-day analogues exhibit significantly higher CAPE, a higher freezing level, and similar deep-layer shear, yielding larger hail probability and size. These results indicate that human-induced warming likely enhanced the hailstorm severity in this synoptic setting.

How to cite: Faranda, D. and Alberti, T.:   Investigating the Role of Climate Change in the 3 May 2025 Western Europe Hailstorm Using Atmospheric Analogues, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2862, https://doi.org/10.5194/egusphere-egu26-2862, 2026.

Thunderstorm activity and associated turbulence pose significant operational challenges for major airports, especially in the context of a changing climate. This study analyzes a high impact winter convective event that forced delays and cancellations at the Rome-Fiumicino airport. We investigate how the synoptic conditions of similar events have evolved over the past five decades (1974–2024) using reanalysis data and a pattern analog approach. We compare atmospheric configurations from the past (1974-1999) and recent (1999-2024), focusing on key parameters related to convection and turbulence. For similar synoptic configurations, our results show an increase in Convective Available Potential Energy (up to 20%), low-level vertical wind shear (up to 20–25%), and turbulence (up to 25-30 %) near Rome-Fiumicino airport in the more recent period, indicating a greater potential for organized convection and turbulence. The analysis of vertical atmospheric profiles reveals enhanced wind shear and turbulence especially in the lower troposphere (0-3 km), with implications for mechanical turbulence during aircraft approach and departure. At Rome-Fiumicino airport, the number of fog and thunderstorms during similar synoptic patterns is increased (from 1 to 4), average approaching visibility decreased from 10 to 7 km, stronger surface winds (from 10 to 15 km/h) are observed, with also increases in average temperatures (from 11 to 13 °C). Finally, using a multinomial logistic model we show that hazardous weather events, particularly thunderstorms and hail, are becoming more frequent for similar recent events (from 2% to 6% annual occurrence). These trends are linked to both human-driven climate change and long-term variations in large-scale modes of natural variability. 

How to cite: Alberti, T. and Faranda, D.: Was the 13 December 2024 severe thunderstorm over Rome-Fiumicino airport intensified by climate change?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2952, https://doi.org/10.5194/egusphere-egu26-2952, 2026.

EGU26-3128 | ECS | Orals | NP1.3

Heatwave-generating Rossby waves and the persistence of temperature extremes in a changing climate 

Wolfgang Wicker, Emmanuele Russo, and Daniela Domeisen

The frequency and duration of hot extremes is projected to increase over the coming decades. It remains, however, unclear to what extent persistent surface temperature extremes require an anomalously persistent circulation in the upper troposphere. To shed more light on this relationship, we combine idealized model experiments with reanalysis data and assess the zonal phase speed of Rossby waves as a proxy for circulation persistence. In particular, we compare the climatological-mean phase speed spectrum to the properties of heatwave-generating Rossby wave packets.

In the idealized model without thermodynamic feedbacks, a phase speed increase in response to a localized thermal forcing reduces the frequency of heatwaves. Reanalysis data for the Southern hemisphere mid-latitudes shows a similar and significant phase speed increase from the 1980s until today. However, the observed mean phase speed increase does not apply to heatwave-generating Rossby waves and hence does not contribute to a change in heatwave frequency. The Northern hemisphere, on the other hand, does not yet show a clear phase speed trend in reanalysis. But with continued global warming, we expect an acceleration of heatwave-generating Rossby waves and a reduced upper-tropospheric forcing to persistent temperature extremes in the future.

How to cite: Wicker, W., Russo, E., and Domeisen, D.: Heatwave-generating Rossby waves and the persistence of temperature extremes in a changing climate, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3128, https://doi.org/10.5194/egusphere-egu26-3128, 2026.

EGU26-3562 | ECS | Orals | NP1.3

Validation of reanalysis products for extreme event attribution at regional and national levels 

Claire Bergin, Clair Barnes, Lionel Swan, Friederike Otto, and Peter Thorne

The WASITUS project was established to build towards an operational event attribution capability for Ireland. The project’s aim is to deep dive into the effect climate change has on extreme weather events at a national level, while also providing additional support to international attribution groups such as project collaborators; World Weather Attribution. 

By focusing on smaller national scales, and investigating data products used in event attribution, attribution studies can become more accurate and offer deeper insight for local responders and policy makers. A main focus of the WASITUS project is to take advantage of the small geographical size of Ireland and work directly with end-users to better understand how event attribution can help them prepare for future changes in extreme weather. These end-users include members of the public, local representatives, and national policy makers. This directly links attribution with real-world planning and damage mitigation measures.

Focusing on the data side of event attribution, most datasets used, whether reanalysis or models, have been tested at large regional or continental scales. However, we have found that the reanalysis data for Ireland, an island nation on the western boundary of most European datasets, is not as accurate as the data over continental Europe. This is quite possibly the case for other nations globally, where a variety of geographical and observational factors may have led to reanalysis products inaccurately representing the weather and climatology. As Ireland sits on the East of the Atlantic ocean, it is prone to weather threats of marine origin. Therefore, it is important to question the data used in creating the reanalysis and model products for Ireland as changing climate trends impact Ireland in different ways to the rest of Europe. 

A particular issue found for reanalysis products is their retrospective extension to earlier decades. To combat this potential issue, we are developing a toolbox to ascertain if reanalysis products reliably characterise the temperatures experienced in a given region for the entirety of the available time-series. The toolbox also aims to identify if shorter subsets of the entire reanalysis timeseries better represent the changing climate than the full dataset. Focusing on ERA5 daily maximum and minimum temperature data over the Republic of Ireland, station observations are being statistically compared to location-specific reanalysis data. While the initial focus will be temperature in Ireland, this toolbox should be readily adaptable for use in different regions globally, as well as on different meteorological parameters, provided sufficient long-term records are available.

In future, it is hoped that other national attribution capabilities, which are being newly formed, can collaborate and aid one another in conducting analysis and report writing. National groups also allow for further research into the methods used for extreme event attribution, where a focus can be placed on improving and expanding the existing attribution capability. In addition, time and focus placed on smaller geographical regions allows for data used in attribution analysis to be thoroughly quality controlled and checked.

How to cite: Bergin, C., Barnes, C., Swan, L., Otto, F., and Thorne, P.: Validation of reanalysis products for extreme event attribution at regional and national levels, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3562, https://doi.org/10.5194/egusphere-egu26-3562, 2026.

EGU26-3580 | Orals | NP1.3

Atmospheric drivers and thermodynamic controls of precipitation variability in North Africa 

Meryem Tanarhte, Andries-Jan De Vries, Georgios Zittis, Moshe Armon, Assaf Hochman, Andreas Karpasitis, Dimitris Kaskaoutis, and Samira Khodayar

Precipitation variability across North Africa spans a wide range of timescales and climatic regimes, from Mediterranean winter precipitation to Saharan convective systems, yet its underlying drivers remain incompletely understood. This contribution synthesizes current knowledge on the atmospheric and surface drivers of precipitation variability in North Africa, drawing on evidence from observations, reanalyses and climate simulations from the Holocene to future projections.

We review the role of large-scale circulation modes, together with synoptic-scale processes such as Rossby wave breaking, cut-off lows, and cyclogenesis, in shaping interannual variability and extreme precipitation events along the Mediterranean coast. Further south, seasonal dynamics linked to the Saharan Heat Low, moisture transport, and land–atmosphere coupling modulate the intermittency and intensity of precipitation in arid regions. Holocene evidence highlights the sensitivity of North African hydroclimate to external forcing and land-surface feedbacks, while also illustrating limits to direct analogy with anthropogenic greenhouse-gas forcing. Future projections indicate that uncertainty in precipitation change is dominated by internal variability and circulation responses, with more robust signals emerging in variability and extremes than in mean precipitation.

As precipitation variability constitutes a climate hazard in its own right, understanding its atmospheric and thermodynamic drivers is central to assessing drought–flood dynamics and their implications for water resources, ecosystems, and human systems across North Africa.

How to cite: Tanarhte, M., De Vries, A.-J., Zittis, G., Armon, M., Hochman, A., Karpasitis, A., Kaskaoutis, D., and Khodayar, S.: Atmospheric drivers and thermodynamic controls of precipitation variability in North Africa, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3580, https://doi.org/10.5194/egusphere-egu26-3580, 2026.

EGU26-5518 | Orals | NP1.3

Can tropospheric configurations linked to the onset or aftermath of polar vortex decelerations be distinguished from climatology? 

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

Wintertime stratospheric circulation in the Northern Hemisphere is dominated by a strong and persistent westerly polar vortex. However, every one to two years, this system undergoes a strong disruption associated with a fast deceleration or even a reversal, accompanied by a massive warming of the polar stratosphere. The tropospheric impacts of these extreme events, commonly referred to as “sudden stratospheric warmings” (SSWs) are well documented, but their precursors and subsequent responses in the troposphere remain frustratingly difficult to categorize systematically. Using recent advances in dynamical systems theory applied to the atmosphere, we analyze from a general point of view, the relationship between very anomalous stratospheric states and tropospheric configurations. We find that highly anomalous geopotential configurations at 10 hPa are unequivocally associated with the occurrence of a strong stratospheric vortex deceleration. However, no distinctive tropospheric patterns can be identified either prior to or following these events. This suggests that both tropospheric precursors and responses to extreme vortex decelerations are fundamentally nonspecific and in consequence, they could be statistically indistinguishable from the background tropospheric variability.

How to cite: Gallego, D., Álvarez-Castro, C., Faranda, D., and Peña-Ortiz, C.: Can tropospheric configurations linked to the onset or aftermath of polar vortex decelerations be distinguished from climatology?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5518, https://doi.org/10.5194/egusphere-egu26-5518, 2026.

EGU26-7152 | ECS | Orals | NP1.3

Extreme precipitation changes in relation to urbanization 

Alice Guccione, Paolo Bassi, Fabien Desbiolles, Matteo Borgnino, Fabio D'Andrea, and Claudia Pasquero

The rising frequency of extreme precipitation is a major concern linked to climate change, commonly associated with increased atmospheric water vapor due to global warming. In densely populated areas, intense rainfall has particularly severe impacts, with urbanization amplifying extreme weather through changes in land surface and local atmospheric conditions.  As attribution science increasingly informs climate policy, it is crucial to discern the extent to which shifts in extreme event probability stem from global versus local anthropogenic drivers. This study analyzes multi-decadal daily precipitation records alongside urbanization indices. In line with previous research, results show a general rise in extreme rainfall frequency, with more intense events exhibiting a larger increase. Analysis of population and urban development metrics reveals that the increase is notably smaller in rural areas, suggesting that the rise attributable to local urban development is of the same order of magnitude as that resulting from global warming. This result is shown to be associated with the urban amplification of convective updraft intensification.

How to cite: Guccione, A., Bassi, P., Desbiolles, F., Borgnino, M., D'Andrea, F., and Pasquero, C.: Extreme precipitation changes in relation to urbanization, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7152, https://doi.org/10.5194/egusphere-egu26-7152, 2026.

EGU26-7744 | Orals | NP1.3

Scale-by-scale two-point statistics in WRF Hybrid LES model 

Kazim Sayeed, Clement Blervacq, Manuel Fossa, Nicolas Massei, and Luminita Danaila

Atmospheric variability spans interacting regimes set by rotation, stratification, and diabatic forcing. One open question is that diagnosing scale-to-scale energy transfer remains challenging because observations rarely provide complete budget closure. We analyze the June 2019 European heatwave using the Weather Research and Forecasting (WRF) model with a hybrid, scale-adaptive LES closure and five nested domains, resolving horizontal separations from O(102) m to O(106)–O(107) m.

Starting from the governing equations of motion in WRF hybrid vertical coordinate, we derive and appraise generalized two-point, Scale-by-Scale (SbS) budget equations for the second-order moments of horizontal velocity increments, reflecting the kinetic energy at each scale. Whilst equations are written for all scales and any point of the considered domains, their assessment against data is performed in a plane parallel to the ground. SbS energy budget equations account for the inhomogeneity, anisotropy, and all effects present in the first principles. We complement these diagnostics with height-dependent characteristic length scales (Kolmogorov, Taylor, Ozmidov, buoyancy, Rhines and Rossby deformation).
We show results for two cases:
i) In the free troposphere, where the SbS kinetic-energy budget is dominated by the advective term (reflecting non-linear interactions and energy transfer), which is balanced by the pressure-gradient contributions. Radial integration of the advective term reproduces the third-order structure function and exhibits a sign reversal near r ∼ 105 m, reflecting transitions between downscale and upscale kinetic energy transfer across mesoscale–synoptic ranges.
ii) In the lower troposphere, we investigate daytime and nocturnal conditions. First, in daytime conditions, the boundary layer exhibits a classical behavior, in which energy is transferred across scales mainly by advective, non-linear effects. Second, for stable stratification during the night, the pressure contribution increases significantly, and the advective transfer adjusts to the pressure-imposed scale dependence, as already noted in the free atmosphere.

These results provide a physically interpretable framework for diagnosing atmospheric cascades across scales and motivate extending SbS budgets to include thermodynamic variables, such as the moist potential temperature and the water vapor content. The latter would allow us to quantify the contributions of radiative and diabatic forcings over short- and long-term timescales, relevant to climate variability.

How to cite: Sayeed, K., Blervacq, C., Fossa, M., Massei, N., and Danaila, L.: Scale-by-scale two-point statistics in WRF Hybrid LES model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7744, https://doi.org/10.5194/egusphere-egu26-7744, 2026.

EGU26-9126 | Posters on site | NP1.3

Cold extremes enduring in a much warmer world 

Eva Holtanova, Senne Van Loon, and Maria Rugenstein

It is the combination of internally induced oscillations and externally forced climate change signals that we observe and feel every day as climate conditions. External forcing can change not only the mean state, but also the internal variability. One of the most important and impactful aspects of variability is the frequency and magnitude of extremes. Even though the cold extremes are expected to warm, they can still have severe impacts on society and ecosystems, which have adapted to a warmer climate. We investigate how the internal variability of winter temperature might change under stronger radiative forcing. For this purpose, we utilize two different datasets: a set of LongRunMIP simulations, analyzing near-equilibrium conditions under preindustrial and abrupt 4xCO2 forcings, and transient large ensemble simulations comparing the historical and scenario periods (the end of the 21st century under RCP8.5/SSP5-8.5 socio-economic pathways). We focus on northern middle latitudes (40 – 70 ° of latitude). In this region, the near-surface climate is largely influenced by atmospheric circulation, including various large-scale modes of variability. A change in the shape of the temperature distribution can then point to a fundamental change in climate-governing processes. It has been argued that increasing winter mean temperatures would be accompanied by a decrease in variance, as day-to-day temperature variations are induced by the occurrence of synoptic-scale weather systems, and in warmer climates, this is expected to decline. Our study provides new insights, showing that the variance shrinking is spatially heterogeneous. We further concentrate on the skewness of the temperature distribution and investigate the changes in the lengths of the cold and hot tails, which are related to the changes in variance. In many mid-latitude regions, the skewness is decreasing, and the cold tail is shrinking at a slower rate than the hot tail, implying enduring cold extremes, even in climatic states much warmer than those we are familiar with.  

How to cite: Holtanova, E., Van Loon, S., and Rugenstein, M.: Cold extremes enduring in a much warmer world, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9126, https://doi.org/10.5194/egusphere-egu26-9126, 2026.

EGU26-9245 | Orals | NP1.3

How to compute extreme cold levels to design power plants in the climate change context?  

Sylvie Parey, Thi Thu Huong Hoang, and Benoit Guisnel

 The expected impact of climate change on temperature extremes is an increase in both the frequency and intensity of heat waves, while cold waves are expected to become less frequent and associated with milder cold temperatures. However, cold waves cannot be ruled out, as cold temperatures similar to those experienced in the past can still occur, at least in the near future, albeit with a lower probability.

While many studies have focused on estimating hot extremes in the context of non-stationary climate change, fewer have addressed the estimation of cold extremes, which must be considered for the design of new installations. Unlike hot extremes, which will intensify over time, the coldest values that might affect existing or planned installations are expected to occur now or in the very near future.

Temperature extremes exhibit different types of non-stationarities: a seasonal cycle, the human-induced climate change trend, and interannual to decadal variability. The seasonal cycle is commonly handled by selecting the season prone to the analyzed extremes. Various methods have been proposed to account for the trend due to human-induced climate change in extreme value estimations, either by considering trends in the parameters of statistical extreme value distributions (Coles, 2001; Parey et al., 2007; Gilleland and Katz, 2016; Barbaux et al., 2025, among others) or by computing a reduced variable whose extremes can be considered stationary and then back-transformed (Parey et al., 2013, 2019; Mentachi et al., 2016). However, for cold extremes, interannual variability generally plays a more significant role.

Therefore, in this study, we propose and test an approach to infer extreme cold values representative of the current climate by combining extreme deviations from the average winter mean and variance, as observed during the coldest winters in the past, with the average conditions of current winters. The methodology will first be described then illustrated with examples.

 

References:

Coles S (2001) An introduction to statistical modelling of extreme values, Springer Series in Statistics. Springer, London

Parey S, Malek F, Laurent C, Dacunha-Castelle D (2007) Trends and climate evolution: statistical approach for very high temperatures in France. Clim Change 81:331–352. https://doi.org/10.1007/s10584-006-9116-4

Gilleland, E., & Katz, R. W. (2016). extRemes 2.0: An Extreme Value Analysis Package in R. Journal of Statistical Software72(8), 1–39. https://doi.org/10.18637/jss.v072.i08

Occitane Barbaux, Philippe Naveau, Nathalie Bertrand, Aurélien Ribes, Integrating non-stationarity and uncertainty in design life levels based on climatological time series, Weather and Climate Extremes, Volume 50, 2025,100807, ISSN 2212-0947, https://doi.org/10.1016/j.wace.2025.100807.

Parey S, Hoang TTH, Dacunha-Castelle D (2013) The importance of mean and variance in predicting changes in temperature extremes. J Geophys Res Atmos 118:8285–8296. https://doi.org/10.1002/jgrd.50629

Parey, S., Hoang, T.T.H. & Dacunha-Castelle, D. Future high-temperature extremes and stationarity. Nat Hazards 98, 1115–1134 (2019). https://doi.org/10.1007/s11069-018-3499-1

Mentaschi, L., Vousdoukas, M. I., Voukouvalas, E., Sartini, L., Feyen, L., Besio, G., & Alfieri, L. (2016). The transformed-stationary approach: a generic and simplified methodology for non-stationary extreme value analysis. Hydrology and Earth System Sciences, 20(9), 3527–3547. https://doi.org/10.5194/hess-20-3527-2016

 

How to cite: Parey, S., Hoang, T. T. H., and Guisnel, B.: How to compute extreme cold levels to design power plants in the climate change context? , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9245, https://doi.org/10.5194/egusphere-egu26-9245, 2026.

EGU26-11777 | Orals | NP1.3

Understanding Complexity to Anticipate Maladaptation: A System Dynamics Approach to Climate Extremes Adaptation with Climate Services 

Riccardo Biella, Luigia Brandimarte, Maurizio Mazzoleni, and Giuliano Di Baldassarre

The risk of extreme climate events is increasing due to the compounding effects of climate change and the increasing dependence on natural resources, with impacts that cascade through ecosystems, livelihoods, and institutions long after the event itself. Climate services are therefore increasingly central to adaptation, providing information that helps anticipate hazards, guide preparedness, and support response. Yet, adaptation can often turn maladaptive when it unintentionally shifts risk to other groups, degrades ecological buffers, or locks systems into trajectories that increase their long-term vulnerability. Climate services rarely account for these unintended consequences, despite their centrality in what decisions can be taken and by whom. Against this backdrop, our contribution presents a methodological framework that integrates system thinking and system dynamics modelling to anticipate how climate services shape long-term socio-ecological outcomes of climate extremes, including the risk of maladaptation.

Our framework combines four elements. First, we use system archetypes to identify recurring maladaptive patterns relevant to extremes’ impacts, such as risk shifting across space or social groups, and “fixes” that reduce immediate losses while degrading ecological resilience. Second, these dynamics are refined through a stakeholder-led iterative process. Third, maladaptation risk and adaptation trade-offs are evaluated and described. Fourth, these dynamics are formalized in a system dynamics model to test different climate information scenarios.

Our application of this framework shows that different typologies of climate services can influence long-term impact trajectories by influencing what risks are prioritized, which measures are selected, and who is able to act. Additionally, under increasing climate variability and compounding shocks, these dynamics become more pronounced, increasing the likelihood that short-term coping undermines long-term resilience. Consequently, accessible and long-term climate services become pivotal in ensuring sustainable adaptive strategies benefitting all stakeholders.

By linking climate services to the complex, socio-ecological impact of climate extremes, this approach lays the groundwork for testing the risk of maladaptation in the development of climate services and adaptation strategies, supporting equitable and durable disaster impact reductions.

How to cite: Biella, R., Brandimarte, L., Mazzoleni, M., and Di Baldassarre, G.: Understanding Complexity to Anticipate Maladaptation: A System Dynamics Approach to Climate Extremes Adaptation with Climate Services, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11777, https://doi.org/10.5194/egusphere-egu26-11777, 2026.

EGU26-12488 | ECS | Orals | NP1.3

Characterization of aviation turbulence associated with Mediterranean tropical-like cyclones (Medicanes) 

Marialuisa Simone, Sergio Servidio, Mario Marcello Miglietta, and Tommaso Alberti

The Mediterranean is a climatologically sensitive region due to its transitional position between the arid subtropics and the wetter mid-latitudes. In recent years, Mediterranean tropical-like cyclones, or Medicanes, have gained increasing attention. These rare baroclinic cyclones that evolve in their mature stage into vortices with structural characteristics similar to tropical cyclones. Although they occur only a few times per decade, Medicanes can produce severe socio-economic impacts through intense precipitation, strong winds, and coastal flooding. 

Observational and modeling studies indicate that rising sea surface temperatures may affect Medicane evolution, potentially leading to stronger storms. Understanding their dynamics is therefore important not only for climatology but also for operational sectors such as aviation, which are directly exposed to atmospheric hazards. While the surface impacts of Medicanes have been widely studied, their influence on upper-tropospheric conditions, particularly turbulence relevant to aviation, remains poorly documented. In-flight encounters with turbulent eddies represent a major aviation hazard, often resulting in injuries, aircraft damage, and economic losses to airlines. 

This study presents the first systematic investigation of aviation-scale turbulence associated with eleven Medicanes that occurred between 1996 and 2023. The analysis is based on three empirical turbulence diagnostics (TI1, TI2, and TI3), commonly used to identify synoptic-scale patterns conducive to shear-induced turbulence. These indices, derived from the ERA5 reanalysis dataset, are computed for each Medicane across the 900–200 hPa layer and as a function of radial distance from the cyclone center, with the aim of assessing how turbulence conditions within Medicanes evolve in a changing climate.

How to cite: Simone, M., Servidio, S., Miglietta, M. M., and Alberti, T.: Characterization of aviation turbulence associated with Mediterranean tropical-like cyclones (Medicanes), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12488, https://doi.org/10.5194/egusphere-egu26-12488, 2026.

EGU26-12606 | ECS | Posters on site | NP1.3

Attribution of the Impacts of the 2024 Extreme Floods in Rio Grande do Sul, Brazil, to Climate Change  

Mireia Ginesta, Leonardo Laipelt, Benjamin Franta, and Rupert F. Stuart-Smith

Extreme flood events are among the most damaging climate-related hazards, with significant human and socio-economic impacts. Understanding the extent to which anthropogenic climate change influences both the physical characteristics and impacts of such events is important for supporting policymakers in risk management and adaptation, informing loss and damage mechanisms, and raising public awareness of the impacts of climate change. Here, we apply a circulation-analogue attribution approach to quantify the impacts of climate change on flooding, extending the use of dynamical analogues from hazard attribution to impact analysis. The framework is designed to work with limited data, making it particularly relevant for data-scarce regions, including much of the Global South.

In late April and early May 2024, extreme flooding affected large parts of the state of Rio Grande do Sul in southern Brazil, being the largest floods ever observed along several regional rivers. The event caused at least 183 fatalities and affected more than 2.3 million people, making it one of the most severe climate-related disasters in Brazil’s history. Weekly rainfall totals exceeded 300 mm across much of the state and 500 mm locally.

In this study, we assess the influence of anthropogenic climate change on the socio-economic impacts of this extreme flood event using a three-step attribution framework. First, we attribute the total event rainfall to climate change by identifying dynamical analogues—events with similar large-scale atmospheric circulation—in single-model initial-condition large ensembles under factual and counterfactual climate conditions. Second, the resulting precipitation signals are used to force a hydrological flood model to quantify climate-induced changes in flood magnitude and spatial extent. Finally, we evaluate the associated socio-economic impacts based on the climate-attributed flood signal.

How to cite: Ginesta, M., Laipelt, L., Franta, B., and Stuart-Smith, R. F.: Attribution of the Impacts of the 2024 Extreme Floods in Rio Grande do Sul, Brazil, to Climate Change , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12606, https://doi.org/10.5194/egusphere-egu26-12606, 2026.

EGU26-13596 | ECS | Orals | NP1.3

Impact of Sudden Stratospheric Warming on the Genesis of Mediterranean Cyclones and Associated Precipitation 

Babita Jangir, Carmen Álvarez-Castro, Cristina Peña Ortiz, David Gallego Puyol, Shira Raveh-Rubin, and Ehud Strobach

Extreme stratospheric polar vortex events, including sudden stratospheric warmings (SSWs) and episodes of strong polar vortex, are known to influence wintertime surface weather by modulating large-scale circulation patterns. While previous studies have primarily focused on their impacts over the North Atlantic and northern Europe, the effects on Mediterranean storm activity remain less well quantified. In this study, we examine the tropospheric response to SSW events from 1979 to 2020, with a particular focus on the associated changes in cyclone activity over the Mediterranean region.

Using a composite analysis of 28 SSW events within the study period, we examine the temporal and spatial evolution of cyclone frequency, genesis density, and associated dynamical fields before and after SSW onset. Seasonal and daily climatological signals are removed to isolate anomalies directly linked to stratosphere-troposphere coupling. Our results show a clear increase in cyclone activity over North Africa and the Atlantic coast of the Iberian Peninsula, associated with increased precipitation over western and southern Europe following SSW events. This is consistent with a southward displacement of the midlatitude jet and storm track. This shift is supported by enhanced upper-level wind speeds, divergence, and potential vorticity anomalies over the region during the post-SSW 2-month period.  Despite the robust composited signal, substantial inter-event variability is observed, indicating that not all SSWs lead to an identical response. These findings highlight the importance of event-to-event differences in determining regional storm impacts.

Overall, this study demonstrates that stratospheric polar vortex disruptions can significantly modulate Mediterranean storms on subseasonal timescales, highlighting the potential value of stratospheric information for enhancing the predictability of wintertime extreme weather over southern Europe and the Mediterranean Basin.

Keywords: Sudden stratospheric warming; polar vortex; Mediterranean cyclones; jet stream; stratosphere–troposphere coupling; subseasonal variability

How to cite: Jangir, B., Álvarez-Castro, C., Peña Ortiz, C., Gallego Puyol, D., Raveh-Rubin, S., and Strobach, E.: Impact of Sudden Stratospheric Warming on the Genesis of Mediterranean Cyclones and Associated Precipitation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13596, https://doi.org/10.5194/egusphere-egu26-13596, 2026.

EGU26-13622 | Orals | NP1.3

Surface temperature extremes mirrored in top of atmosphere radiative fluxes 

Doris Folini and Daniela Domeisen

Using ERA5 re-analysis data, 1950 to 2024, we look at surface temperature extremes, which we define as regions of at least 0.5 million square kilometers where the monthly mean 2m temperature exceeds its 25 year climatological mean by at least 1.5 standard deviations. While heat extremes are overall a topic of intense research, we here target a facet of such extreme events that has been less examined so far: how they manifest in terms of top of atmosphere (TOA) radiative fluxes. For the short- and long-wave TOA fluxes associated with such extreme events, we find typically enhanced values. This may be expected, given that mid-latitude heat waves are often accompanied by clear skies. For the TOA net energy flux, we find typically negative values. Spatially more extended extreme events tend to be associated with stronger temperature anomalies. Individual extreme events may deviate from these general tendencies. For selected extremes, daily ERA5 re-analysis data are examined. For the period 2001 to 2024, TOA fluxes from ERA5 re-analysis are compared to CERES satellite data.

How to cite: Folini, D. and Domeisen, D.: Surface temperature extremes mirrored in top of atmosphere radiative fluxes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13622, https://doi.org/10.5194/egusphere-egu26-13622, 2026.

EGU26-14086 | Orals | NP1.3 | Highlight

Emerging evidence of Greenland Ice Sheet melt influence on recent Euro-Mediterranean record-breaking heat and convective storms 

Juan Jesús González-Alemán, Marilena Oltmanns, Sergi González-Herrero, Frederic Vitard, Markus Donat, Francisco Doblas-Reyes, David Barriopedro, Jacopo Riboldi, Carlos Calvo-Sancho, Bernat Jiménez-Esteve, Pep Cos, and Michael Wehner

In recent decades, the Euro–Mediterranean region has experienced a marked increase in catastrophic summer climate extremes, including persistent record-breaking atmospheric and marine heatwaves, and destructive convective events such as long-lived mesoscale convective systems (derecho) and supercells with unparalleled hail-size. All these have provoked severe socioeconomic, ecological and human impacts. While these phenomena are often studied separately, their frequent co-occurrence suggests the influence of common large-scale circulation drivers, which remain actively debated.  

Building on recent work linking North Atlantic freshwater anomalies to downstream atmospheric circulation responses, this ongoing study explores whether part of the recent European summer climate signal may be influenced by remote hemispheric-scale forcing associated with Greenland Ice Sheet mass loss, which has also coincidentally accelerated in recent decades due to anthropogenic influences. This linkage was not initially targeted but emerged unexpectedly from exploratory diagnostics motivated by broader investigations of North Atlantic variability. Preliminary results indicate that periods of enhanced summer Greenland melt tend to coincide with subsequent anomalous spring–summer circulation patterns over the Euro-Atlantic sector that favour persistent ridging and blocking-like conditions over the Euro-Mediterranean region. Such circulation states are consistent with environments conducive to prolonged heat stress, the development of marine heatwaves, and subsequent severe convective outbreaks.

Initial comparisons with global climate models from CMIP6 suggest that this potential pathway is poorly represented, possibly due to limitations in simulating localized freshwater forcing and its coupled atmosphere–ocean effects, which indicates that current projections of future climate may be underestimating these impacts. Our findings would point out Greenland melting as a previously unreported major driver of spring-summer large-scale circulation changes. Incorporating these processes could then be essential for forecasts systems and long-term projections, likely posing a significant gap in our ability to project future risk. Ongoing work focuses on testing the robustness of this emerging signal, clarifying its relevance relative to other known drivers of European summer extremes and exploring its hemispheric-scale reach.

How to cite: González-Alemán, J. J., Oltmanns, M., González-Herrero, S., Vitard, F., Donat, M., Doblas-Reyes, F., Barriopedro, D., Riboldi, J., Calvo-Sancho, C., Jiménez-Esteve, B., Cos, P., and Wehner, M.: Emerging evidence of Greenland Ice Sheet melt influence on recent Euro-Mediterranean record-breaking heat and convective storms, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14086, https://doi.org/10.5194/egusphere-egu26-14086, 2026.

EGU26-14429 | ECS | Orals | NP1.3

From Mapping to Action: ADAPT-TOOLS and What We Learn from the Mediterranean CCA Toolscape 

Athanasios Tsilimigkras, Christian Pagé, Milica Tošić, Irida Lazić, Elisa Savelli, and Aristeidis Koutroulis and the FutureMed WG2

Climate change adaptation (CCA) is supported by a rapidly expanding ecosystem of decision-support systems, risk and vulnerability assessments, data portals, guidance frameworks, and early-warning services. Yet selecting an appropriate tool for a specific decision context remains difficult because tool information is often fragmented, inconsistently described, and not searchable using the metadata that practitioners actually need (e.g., sector, scale, user group, methods, outputs, usability, cost, and geographic scope). Within the FutureMed COST Action, WG2 has compiled a structured inventory of Mediterranean-relevant CCA tools and developed a shared criteria systematization to describe who tools are intended to serve, what they support, and how they are applied in practice. Insights emerging from this collaborative effort highlight that availability is not the only challenge: tool–context alignment is frequently unclear, tools often operate in isolation with limited guidance for selection, and the way tools define their spatial applicability may follow administrative rather than physical boundaries. Multilingual support and pathways for incorporating local data and knowledge are uneven. These patterns motivate the need for an operational resource that makes tools legible, comparable, and easier to navigate for real-world use.

We present ADAPT-TOOLS, a live database and web platform that translates a fragmented inventory into actionable discovery through structured metadata and faceted exploration. Tools are organized using a harmonized taxonomy spanning several aspects: intended user groups (policy, local government, private sector, NGOs, academia), sector focus, tool type, political and physical target scales, temporal horizon and resolution, methodological approach, data utilization, output types, accessibility/usability, validation and reliability signals, cost and support characteristics, and geographic applicability. Users can combine filters (OR within filters, AND across filters) to rapidly narrow from broad categories to tools matching their constraints, while dedicated tool pages support transparent comparison and adoption.

Technically, the platform is implemented as a containerized stack with a relational backend and a web interface. A reproducible ingestion pipeline converts structured inventories into relational tables, enabling systematic updates and maintainable curation workflows. To support sustained evolution and community engagement, ADAPT-TOOLS includes a moderated “Suggest a Tool” workflow that collects structured submissions for review before integration, enabling continuous expansion while preserving data quality. The platform is publicly deployed at adapt-tools.org. By linking community mapping to an operational platform, ADAPT-TOOLS supports evidence-informed and more context-aware adaptation planning across the Mediterranean and beyond.

Acknowledgments

This study is based on work from COST Action CA22162 “FutureMed: A Transdisciplinary Network to Bridge Climate Science and Impacts on Society” (FutureMed), supported by COST (European Cooperation in Science and Technology).

How to cite: Tsilimigkras, A., Pagé, C., Tošić, M., Lazić, I., Savelli, E., and Koutroulis, A. and the FutureMed WG2: From Mapping to Action: ADAPT-TOOLS and What We Learn from the Mediterranean CCA Toolscape, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14429, https://doi.org/10.5194/egusphere-egu26-14429, 2026.

EGU26-14636 | Orals | NP1.3

EO4Multihazards: Earth Observation for high-impact multi-hazard science 

Egor Prikaziuk, Jacopo Furlanetto, Bastian van den Bout, Giuliano Boscarin, Margarita Huesca, Edoardo Albergo, Marinella Masina, Davide Mauro Ferrario, Margherita Maraschini, Silvia Torresan, Cees van Westen, Irene Manzella, and Carlos Domenech

Earth Observation for high-impact multi-hazard science (EO4Multihazards) was a European Space Agency (ESA) project that developed methodologies for risk (hazard, vulnerability, exposure) and impact assessment with the help of Earth Observation (EO) data. We assessed cascading and compound events and developed impact chains for four case studies in Italy (upper and lower Adige river basin), the United Kingdom and Dominica, a Caribbean Small Island Developing State. This abstract presents the fifth, so-called “transferability”, case study, where developed methodologies were applied in an area with limited ground validation data, Senegal. Droughts, heatwaves, floods and fires were analysed for the regions specified by stakeholders. The risk for the population and the impact on agricultural yields were assessed in the riskchanges.org platform. The vulnerability components were shown to be the most challenging and ground-data demanding. Visit our website to explore other outputs, such as a whole Europe event database and case study geostories https://eo4multihazards.gmv.com/.

We acknowledge support from the EO4Multihazards project (Earth Observation for high-impact multi-hazards science), contract number 4000141754/23/I-DT, funded by the European Space Agency and launched as part of the joint ESA-European Commission Earth System Science Initiative.

How to cite: Prikaziuk, E., Furlanetto, J., van den Bout, B., Boscarin, G., Huesca, M., Albergo, E., Masina, M., Mauro Ferrario, D., Maraschini, M., Torresan, S., van Westen, C., Manzella, I., and Domenech, C.: EO4Multihazards: Earth Observation for high-impact multi-hazard science, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14636, https://doi.org/10.5194/egusphere-egu26-14636, 2026.

EGU26-14907 | Posters on site | NP1.3

Exploring Sudden Stratospheric Warming Dynamics: A Data-Driven Analysis Using a Low-Dimensional Stochastic Model 

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

Sudden Stratospheric Warmings (SSWs) are extreme atmospheric events characterized by a rapid weakening or breakdown of the polar vortex, often followed by profound impacts on surface weather. These include abrupt temperature anomalies, shifts in large-scale circulation patterns, modulation of jet streams, and an increased likelihood of cold-air outbreaks and altered storm tracks at mid-latitudes. As a result, SSWs play a pivotal role in shaping the occurrence and intensity of extreme weather events across the Northern Hemisphere. Although low-dimensional models have proven instrumental in elucidating the fundamental wave–mean flow interactions underlying SSWs, their ability to faithfully reproduce the full complexity, variability, and predictability of real atmospheric dynamics remains limited.

In this study, developed within the framework of the VORTEX project, we introduce a novel data-driven methodology to systematically assess the realism and predictive skill of low-dimensional models in simulating SSW dynamics. Our approach is based on two complementary metrics, dimension and persistence, which quantify, respectively, the effective dynamical complexity and the temporal coherence of the system. Together, these metrics provide a robust framework to evaluate how well simplified models capture the essential features of observed stratospheric variability.

Using this methodology, we investigate the sensitivity of SSW dynamics to large-scale tropospheric forcing and stochastic variability, both of which are known to be key contributors to vortex destabilization. To this end, we propose a stochastic low-order model that couples the Holton–Mass equations, representing wave–mean flow interactions, with a Langevin formulation that accounts for the bistable nature of the polar vortex.

Our results demonstrate that both the frequency and dynamical characteristics of SSWs exhibit a pronounced sensitivity to changes in tropospheric wave forcing and noise intensity. We identify critical thresholds beyond which the probability of vortex breakdown increases sharply, offering a mechanistic interpretation of the observed intermittency and variability of SSW events. These findings provide new insight into stratosphere–troposphere coupling and highlight the potential of data-driven diagnostics to bridge the gap between conceptual models and the complexity of the real atmosphere.

How to cite: Alvarez-Castro, C., Peña-Ortiz, C., Gallego, D., and Faranda, D.: Exploring Sudden Stratospheric Warming Dynamics: A Data-Driven Analysis Using a Low-Dimensional Stochastic Model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14907, https://doi.org/10.5194/egusphere-egu26-14907, 2026.

EGU26-15294 | ECS | Orals | NP1.3

Bridging Climate-Health Attribution Science and Health-Sector Practice 

Bianca Corpuz, Sadie Ryan, Rupert Stuart-Smith, Mauricio Santos Vega, Gabriel Carrasco-Escobar, Tatiana Marrufo, James Chirombo, Joy Shumake-Guillemot, Ana Vicedo-Cabrera, and Rachel Lowe

Attribution science has made substantial progress in quantifying the influence of anthropogenic climate change on extreme events, yet its application to human health outcomes remains limited and difficult to operationalize for health-sector practitioners. Methodological complexity, fragmented guidance, and challenges in interpreting and communicating results hinder the uptake of climate-health attribution evidence in public health decision-making. We present the development of a structured, accessible resource designed to support health-sector engagement with climate-health attribution and its application in public health decision-making, within the TACTIC (HealTh ImpAct ToolkIt for Climate change attribution) project funded by the Wellcome Trust. This work is designed as an accessible, practice-oriented resource that complements technical methodological materials, supporting users who wish to understand or engage with climate-health attribution studies. While primarily targeting public health professionals and health agencies, it is also intended to be useful for researchers, policy advisors, and communicators working at the climate-health interface. This work synthesizes existing evidence and emerging best practices in health impact attribution and is structured around key practical questions: when attribution is feasible for specific climate hazards and health outcomes; what data, assumptions, and methods are required; how results should be interpreted and communicated; and how uncertainty and limitations should be conveyed. Its development is informed by stakeholder engagement, community input, and applied case studies in climate-vulnerable regions, ensuring relevance across diverse geographical and resource contexts. By translating complex attribution concepts into clear, actionable guidance, this work aims to build capacity, support evidence-informed public health action, and strengthen the integration of climate-health attribution science into policy and practice.

How to cite: Corpuz, B., Ryan, S., Stuart-Smith, R., Santos Vega, M., Carrasco-Escobar, G., Marrufo, T., Chirombo, J., Shumake-Guillemot, J., Vicedo-Cabrera, A., and Lowe, R.: Bridging Climate-Health Attribution Science and Health-Sector Practice, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15294, https://doi.org/10.5194/egusphere-egu26-15294, 2026.

The Eastern Mediterranean is a well-established climate change hotspot, where intensifying hydrological extremes increasingly translate into high-impact weather conditions with cascading societal consequences. While long-term changes in mean atmospheric moisture are relatively well documented, much less is known about the evolution of extreme moisture states that act as precursors to severe precipitation, flooding, and compound hydroclimatic hazards.

In this study, we investigate the extreme behaviour of precipitable water vapour (PWV) using homogenised, high-frequency GNSS-derived observations from a dense network located in the Eastern Mediterranean transition zone. To ensure climate-quality consistency, the dataset was processed following internationally recognised standards, including IGS Repro3 strategies, covering the period 2010–2024. Moving beyond conventional trend-based analyses, we employ a non-stationary Extreme Value Theory (EVT) framework, combining Generalised Extreme Value (GEV) and Peak-Over-Threshold (POT) approaches to characterise the tails of the PWV distribution. This enables an assessment of changes in the magnitude, frequency, and persistence of rare moisture extremes under ongoing warming, independent of mean climatological shifts.

Return levels corresponding to different recurrence intervals are estimated to provide observational constraints on extreme atmospheric moisture scaling and its consistency with theoretical Clausius–Clapeyron expectations. The statistical results are further interpreted in the context of large-scale atmospheric drivers using ERA5 reanalysis data, shifting the focus from describing atmospheric states to identifying weather conditions conducive to high-impact hydroclimatic outcomes.

This contribution directly aligns with the objectives of the FutureMed COST Action (CA22162) by bridging physical climate processes, advanced statistical characterisation of extremes, and impact-relevant indicators of risk. By focusing on extreme moisture states rather than mean conditions, the study supports a shift from describing what the atmosphere is to assessing what weather conditions are likely to do in terms of hydroclimatic impacts, thereby improving the understanding and predictability of high-impact weather in the Eastern Mediterranean region.

How to cite: Zengin Kazancı, S.: Unveiling the Tails of Atmospheric Moisture Extremes in the Eastern Mediterranean: Non-Stationary GNSS-Based Evidence for High-Impact Hydroclimatic Conditions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16534, https://doi.org/10.5194/egusphere-egu26-16534, 2026.

EGU26-17367 | Posters on site | NP1.3

Mediterranean Extreme Events in a changing climate on multiple spatiotemporal scales 

Tommaso Alberti, Johannes de Leeuw, Giovanni Scardino, Federico Siciliano, and Natalia Zazulie

Climate change is changing the statistics and the physics of extreme weather events, leading to increasing impacts from heavy precipitation, floods, droughts, heatwaves, and so on. Thus, attribution of extremes requires a process-based understanding of how large-scale forcing interacts with regional dynamics and thermodynamics. Despite significant progress at global scales, attribution of extremes at regional and local scales remains challenging, particularly in regions where small-scale processes dominate the generation of high-impact events.

The Mediterranean basin is a hotspot for climate change, characterized by land–sea interactions, complex orography, and convective activity. Extreme events in this region are often controlled by small-scale (1–10 km) processes, including atmospheric instability and convective organization. These processes are poorly represented in coarse-resolution climate models, limiting our ability to attribute observed impacts and to assess future risks.

The Mediterranean Extreme Events and Tipping elements in a changing climate on multiple spatiotemporal scales (MEET) project addresses this challenge through a process-oriented, high-resolution framework focused on Mediterranean extremes and their impacts. MEET will identify and classify historical and recent extreme events based on their impacts on key meteorological variables, such as precipitation intensity, near-surface temperature extremes, and damaging winds, and on associated societal and environmental consequences. Physics-informed decomposition techniques combined with advanced statistical methods will be applied to identify analog events across multiple spatiotemporal scales, enabling the detection of changes in event frequency, intensity, and spatial structure. A central component of MEET is the use of convection-permitting climate simulations to explicitly resolve the small-scale dynamics and thermodynamics underlying extreme events in both past and future climates. By linking high-resolution physical processes to observed impacts, MEET aims to advance the attribution of Mediterranean extreme events and to provide a physically consistent basis for improved regional risk assessment under ongoing climate change.

 

Acknowledgements

This research has been carried out with funding from the Italian Ministry of University and Research under the FIS-2 Call.

How to cite: Alberti, T., de Leeuw, J., Scardino, G., Siciliano, F., and Zazulie, N.: Mediterranean Extreme Events in a changing climate on multiple spatiotemporal scales, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17367, https://doi.org/10.5194/egusphere-egu26-17367, 2026.

EGU26-17874 | ECS | Posters on site | NP1.3

Satellite-Based Analysis of Urban Heat Island Dynamics under Extreme Heatwave Conditions and Mitigation Strategies in Thessaloniki 

Marco Falda, Giannis Adamos, Tamara Radenovic, and Chrysi Laspidou

Heatwaves are among the most impactful and rapidly intensifying climate extremes in the Mediterranean region, where rising mean temperatures and the increasing frequency of extreme events interact with urban environments, exacerbating thermal stress. In densely populated cities, the Urban Heat Island (UHI) effect acts as a local amplification mechanism, transforming large-scale atmospheric heatwaves into compound extreme events with significant societal and environmental consequences. This study analyzes the spatial distribution and main controlling factors of extreme surface temperatures during three intense summer heatwaves in Thessaloniki, Greece, with the aim of linking observed geophysical extremes to urban configuration and assessing the potential of mitigation measures. For this aim, we employ LANDSAT 8–9 satellite imagery processed in QGIS to derive high spatial resolution Land Surface Temperature (LST) fields, together with key land-cover indicators such as the Normalized Difference Vegetation Index (NDVI) and the Normalized Difference Built-up Index (NDBI). These remote-sensing products are integrated with urban morphology and land-use data derived from OpenStreetMap (OSM), enabling a detailed characterization of how vegetation cover, building density, and surface materials modulate the urban thermal response under conditions of extreme atmospheric forcing. The results reveal pronounced spatial heterogeneity in LST across the metropolitan area, with persistent hotspots associated with compact historic districts, industrial zones, and highly impervious surfaces. In contrast, urban parks, coastal areas, and neighborhoods with a higher fraction of vegetation exhibit significantly lower surface temperatures, highlighting the role of land–atmosphere interactions and surface energy balance feedbacks in shaping urban-scale thermal extremes. The inverse relationship between NDVI and LST, together with the positive relationship between NDBI and LST, indicates the strong sensitivity of urban surface temperatures to land-cover composition during heatwave conditions. By framing the UHI as an intrinsic component of compound heat extremes, this work bridges observational geophysical analysis with the assessment of urban impacts. We further explore the potential of targeted mitigation strategies, such as the large-scale implementation of green roofs and high-albedo pavements, demonstrating their ability to reduce extreme surface temperatures and to moderate thermal exposure. The findings emphasize the importance of integrating physically grounded, data-driven mitigation measures into standardized urban planning frameworks in order to enhance resilience to future thermal extremes. More broadly, the study contributes to the understanding of how local-scale processes interact with large-scale climate extremes, offering transferable insights for Mediterranean and European cities increasingly exposed to heatwave risk under climate change.

How to cite: Falda, M., Adamos, G., Radenovic, T., and Laspidou, C.: Satellite-Based Analysis of Urban Heat Island Dynamics under Extreme Heatwave Conditions and Mitigation Strategies in Thessaloniki, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17874, https://doi.org/10.5194/egusphere-egu26-17874, 2026.

Extreme precipitation over Europe is often linked to large-scale atmospheric circulation anomalies, yet it remains unclear which dynamical features recur systematically across many independent events, and how their influence evolves with time and altitude. In particular, the extent to which coherent, large-scale dynamical structures act as precursors to extreme rainfall has not been quantified so far beyond traditional composite-based approaches.

Here, we introduce a lagged coupled climate-network framework to investigate the interdependency between extreme precipitation events and atmospheric circulation from a functional climate network perspective. Extreme precipitation events are identified from ERA5 precipitation data by applying a local percentile threshold to daily precipitation sums and represented as binary event series, while two-dimensional fields of additional variables in different atmospheric layers—including geopotential height, relative vorticity, and temperature at multiple pressure levels—are treated as continuous variables. Using point-biserial correlation as statistical association measure between these different types of time series, we construct lagged event–field coupled networks that explicitly distinguish positive and negative statistical associations. Network connectivity is quantified through the cross-degree, which measures how many grid points of surface extreme events are significantly linked to a given atmospheric grid point (and vice versa), thereby emphasizing the recurrence and spatial relevance of circulation features rather than their correlation strength alone.

Our analysis reveals a coherent temporal evolution and vertical structure of circulation coupling to hydrometeorological extremes at the surface. At negative lags, cross-degree patterns are dominated by mid- to upper-tropospheric geopotential height and vorticity anomalies, indicating the recurrent presence of large-scale dynamical features prior to extreme precipitation events. With increasing lag, the coupling progressively shifts toward lower tropospheric levels, suggesting a transition from large-scale circulation influences before the events to near-surface circulation imprints afterward. Spatially, regions of enhanced cross-degree exhibit a systematic west-to-east displacement with changing lag, extending from the western North Atlantic and Greenland sector toward continental Europe. This spatial progression is consistent with downstream evolution along the North Atlantic–European circulation corridor. A pronounced and recurrent signal over the British Isles emerges across multiple variables, highlighting this region as a dynamically relevant area in the large-scale circulation context of European precipitation extremes.

By explicitly quantifying where, when, and at which vertical levels circulation anomalies of the same type recur across many extreme events, our coupled network approach provides a complementary perspective to conventional correlation and composite analyses. Our results demonstrate the potential of coupled functional climate networks to identify robust, recurring circulation patterns associated with extreme precipitation, offering new insights into precursor dynamics, vertical coupling, and large-scale organization of midlatitude extremes without assuming a specific underlying mechanism.

How to cite: Bishnoi, G. and V. Donner, R.: Lagged Coupled Climate Networks for Identifying Recurrent Circulation Patterns Behind Extreme Rainfall in Europe, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18041, https://doi.org/10.5194/egusphere-egu26-18041, 2026.

EGU26-18062 | ECS | Orals | NP1.3

Attribution of Austral Summer Extreme Temperature Events in Antarctica Using a Circulation Analogue Method  

Yuiko Ichikawa, Neven S. Fuckar, Thomas Bracegirdle, and Mireia Ginesta

The global climate system is undergoing rapid changes unprecedented in human history, with increasingly extreme weather events observed across the world. Antarctica is particularly exposed to these changes, with some of the highest warming rates on the planet recorded over West Antarctica in recent decades and emerging warming trends now evident in East Antarctica. Despite this, relatively few studies have focused on the attribution of extreme temperature events in Antarctica, where near-surface temperatures are strongly conditioned by large-scale atmospheric circulation over the continent and the Southern Ocean. 

Here, we apply a circulation-analogue technique for extreme-event attribution to assess how dynamically similar warm extremes have changed over time. We focus on three recent austral-summer warm extremes: the February 2020 heatwave over the Antarctic Peninsula, the March 2022 warm anomaly across East Antarctica, and the March 2015 warm spell on the Peninsula. These short-duration events produced exceptional near-surface temperature anomalies. 

Circulation analogues associated with these events are analysed across two climatic periods: a “past’’ baseline (1948–1986) and a “present’’ period (1987–2025), using two independently developed atmospheric reanalysis products, ERA5 and JRA-3Q. Changes in the occurrence frequency of analogue weather types and in their associated near-surface temperature anomalies provide insight into the influence of anthropogenic climate change on these extremes. The dual-dataset approach offers a more robust basis for attribution, particularly for the pre-satellite era when reanalysis uncertainties and dataset discrepancies are considerable. 

How to cite: Ichikawa, Y., S. Fuckar, N., Bracegirdle, T., and Ginesta, M.: Attribution of Austral Summer Extreme Temperature Events in Antarctica Using a Circulation Analogue Method , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18062, https://doi.org/10.5194/egusphere-egu26-18062, 2026.

EGU26-18393 | ECS | Orals | NP1.3

Interdisciplinary Approaches in the Study of Climate Extremes 

Chenyu Dong and Gianmarco Mengaldo

Climate extremes, including heatwaves, extreme precipitation, tropical cyclones, and related 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 these extremes. 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 climate extremes.

How to cite: Dong, C. and Mengaldo, G.: Interdisciplinary Approaches in the Study of Climate Extremes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18393, https://doi.org/10.5194/egusphere-egu26-18393, 2026.

EGU26-18626 | ECS | Orals | NP1.3

Understanding Shifts in Extreme Precipitation and Synoptic Forces in a Regionalized Framework: The Iberian Peninsula 

Pau Benetó, Jose Antonio Valiente, and Samira Khodayar

Extreme precipitation exhibits pronounced local variations associated with dynamic and thermodynamic changes on synoptic and regional scales under global warming inducing important impacts over main socioeconomic sectors such as agriculture, tourism, health and energy. Local-to-regional variations in extreme precipitation are especially marked on climate change hotspots, such as the Iberian Peninsula, reflecting the complex transition between Atlantic and Mediterranean climate influences and further hindering an accurate assessment of climate change impacts and the development of effective adaptation strategies. Therefore, it is crucial to identify variations in atmospheric dynamics as main drivers of changes in the characteristics of extreme precipitation events (EPEs) on subregional scales to better determine the areas subject to specific changes and improve our understanding of extreme weather events to enhance predictability.

In this context, this study conducted a comprehensive analysis using a precipitation regionalization approach with a high resolution (~5 km) gridded dataset for the period 1951-2021 obtaining 8 precipitation-coherent regions in the Iberian Peninsula. EPEs were characterized over each region, and their evolving atmospheric drivers were identified using an objective synoptic classification method with ERA5 data. Besides, an analysis of variations in EPEs intensity and frequency, as well as changes in the associated synoptic conditions and atmospheric water vapor distributions were assessed.

Our results revealed a generalized mean intensification of EPEs for the study period. Nevertheless, we highlight two different pathways: (i) Atlantic regions presenting a moderate (5-10 %) intensification of extreme precipitation linked to an increase of surface flows and counterposing the observed weakening or northward displacement of upper-level perturbations, and (ii) Mediterranean regions showing a marked (15-25 %) extremization of EPEs associated with vorticity intensification at 500 hPa.  Besides, these variations occur alongside an atmospheric moistening (up to 6 mm in the Ebro region) of the moistest air masses denoting the highly complex interplay between thermodynamic and dynamic factors. We emphasize the importance of regionalized approaches to enhance our comprehension on extreme precipitation over regions with complex topography and, more importantly, the corresponding implications on early warning systems and efficient climate adaptation strategies in climate change hotspots.

How to cite: Benetó, P., Valiente, J. A., and Khodayar, S.: Understanding Shifts in Extreme Precipitation and Synoptic Forces in a Regionalized Framework: The Iberian Peninsula, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18626, https://doi.org/10.5194/egusphere-egu26-18626, 2026.

The analysis of the impacts due to climate extremes, such as extreme precipitation, heatwaves, and tropical cyclones, needs to rely on multimodal data, ranging from complex geophysical fields to textual and visual data.

While recent advances in vision-language models (VLMs) have stimulated interest in multimodal-driven climate analysis, their application to natural hazard analysis is still relatively limited.

In this work, we focus on tropical cyclones, and construct a new framework, namely Visual Object Representation for Tropical Cyclone Extremes and eXtent (VORTEX), a physics-aware, visual abstraction designed to support interpretable vision-language reasoning over hazard fields for tropical cyclones.

VORTEX transforms spatiotemporal reanalysis data associated to tropical cyclones into structured, visually identifiable representations by explicitly encoding cyclone-specific physical properties, including pressure-anchored storm geometry, wind and precipitation intensity extrema, spatial asymmetry, and field-scale footprint.

Building on VORTEX, we construct ClimateFieldQA, a structured evaluation framework for diagnosing VLM reasoning over tropical cyclone hazard fields. ClimateFieldQA comprises 4,978 high-resolution reanalysis heatmaps and 243,922 instruction samples spanning spatial localization, intensity estimation, structural pattern recognition, field-scale extent reasoning, and physical impact analysis.

ClimateFieldQA is designed to expose strengths, limitations, and failure modes of VLM-based reasoning under physically constrained geoscientific settings.

Using ClimateFieldQA, we show that physics-aware visual abstractions systematically improve structure-sensitive reasoning and reduce common interpretation errors observed when VLMs operate on raw hazard fields, highlighting the methodological importance of representation design for climate impact analysis and natural hazard assessment in Earth system science.

How to cite: Xiao, L. and Mengaldo, G.: ClimateFieldQA: Evaluating Vision–Language Models on Tropical Cyclone Hazard Fields with Physics-Aware Visual Abstractions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18916, https://doi.org/10.5194/egusphere-egu26-18916, 2026.

EGU26-18955 | Orals | NP1.3

Sea surface temperature anomalies associated with Mediterranean tropical-like cyclones  

Francisco Pastor, Daniel Pardo-García, and Samira Khodayar

Mediterranean tropical-like cyclones, known as medicanes, are mesoscale systems that develop over the Mediterranean Sea and exhibit structural similarities to tropical cyclones, despite forming under markedly different environmental conditions. Air–sea interactions play a key role in their development and intensification, yet the behaviour of sea surface temperature (SST) before, during, and after medicane events remains insufficiently quantified. 

In this study, we analyse SST anomalies and daily SST variability associated with medicane events using the Copernicus high-resolution Level-4 reprocessed Sea Surface Temperature dataset. Daily SST fields and their day-to-day variations are examined along medicane tracks and surrounding areas and compared against climatological references to assess the SST response to medicane passage. The analysis accounts for differences related to seasonality, medicane development stage, and formation region within the Mediterranean basin. 

Results reveal marked SST anomalies associated with medicane events, with a consistent reduction in daily SST and a pronounced negative anomaly in daily SST variation along the medicane track. The magnitude and spatial extent of these anomalies vary depending on the season and phase of the medicane life cycle, indicating distinct air–sea interaction regimes across different Mediterranean sub-basins. The observed SST cooling is consistent with enhanced surface fluxes and upper-ocean mixing induced by medicane-related wind forcing. 

These findings highlight the role of SST anomalies and short-term SST variability in the evolution and intensification of medicanes and provide new insights into the coupled ocean–atmosphere processes governing these systems. Improved understanding of SST–medicane interactions is essential for better representation of medicane-related hazards and for assessing their potential impacts in a warming Mediterranean, where socio-economic exposure and vulnerability are increasing. 

 

How to cite: Pastor, F., Pardo-García, D., and Khodayar, S.: Sea surface temperature anomalies associated with Mediterranean tropical-like cyclones , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18955, https://doi.org/10.5194/egusphere-egu26-18955, 2026.

EGU26-18974 | ECS | Posters on site | NP1.3

Future Warm–Dry and Warm–Wet Compound Climate Extremes in Mediterranean Metropolitan Areas under Climate Change 

Iliana Polychroni, Maria Hatzaki, Platon Patlakas, and Panagiotis Nastos

The Mediterranean region is widely recognized as a climate change hotspot, as anthropogenic warming is projected to substantially increase air temperatures by the end of the 21st century, together with longer periods of reduced rainfall. The region is likely to experience warmer and drier conditions with significant consequences for human societies, while the intensification of heatwaves is likely to trigger cascading hazards. At the same time, heavy precipitation events during hot periods may become more common, increasing the likelihood of urban flash floods, especially in densely populated metropolitan areas.

Instead of focusing only on single climate extremes,, compound extremes offer a complementary perspective for assessing future climate risks. We analyze two compound climate indices: Warm/Dry (WD) and Warm/Wet (WW) days. The analysis focuses on representative Mediterranean metropolitan areas characterized by high population density and climatic relevance.

The indices are derived from daily mean temperature and precipitation data obtained from an ensemble of CMIP6 climate model simulations. Annual and seasonal frequencies of compound extremes are evaluated for the mid-century (2041–2060) and late-century (2081–2100) periods, relative to a 1995–2014 reference period, under the SSP2-4.5 and SSP5-8.5 scenarios. Results indicate a robust increase in the frequency of Warm/Dry days across all future scenarios, suggesting that Mediterranean climates will increasingly experience concurrent warming and drying. In contrast, Warm/Wet days are scenario-dependent. These findings highlight a dual climate risk for Mediterranean cities, where more frequent prolonged hot and dry conditions coexist with a higher chance of compound heat and heavy precipitation events under high-emission scenarios.

How to cite: Polychroni, I., Hatzaki, M., Patlakas, P., and Nastos, P.: Future Warm–Dry and Warm–Wet Compound Climate Extremes in Mediterranean Metropolitan Areas under Climate Change, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18974, https://doi.org/10.5194/egusphere-egu26-18974, 2026.

EGU26-19076 | ECS | Orals | NP1.3

The exceptional October 2024 flooding in Valencia (Spain): meteorological drivers of an extreme precipitation event 

David Espín, Pau Benetó, and Samira Khodayar

The late-October 2024 flooding in Valencia (eastern Spain) was triggered by an exceptional extreme precipitation event (EPE) associated with a quasi-stationary cut-off low over the western Mediterranean. In this study, we assess the meteorological exceptionality of the October 2024 event by combining a basin-scale, percentile-based catalogue of rainfall extremes with a multi-level diagnosis of thermodynamic and dynamical atmospheric drivers.

Extreme precipitation is analysed using the dense SAIH rain-gauge network covering the Júcar River Basin at hourly and 5-minute temporal resolution for the period 1990–2024. Hourly p99 precipitation thresholds are computed for each station using an autumn (September–November) rolling-hour climatology. Local exceedances above p99 are aggregated into a basin-wide “overall magnitude” index (M), which integrates intensity and spatial footprint. EPEs are identified as continuous periods with M > 0 and ranked according to duration, peak intensities at 1-, 3-, 6-, 12- and 24-hour accumulation periods, cumulative local magnitude, mean excess above threshold, and the number of affected stations. The October 2024 event is contextualised against (i) the seven most extreme autumn EPEs (>p99) over the last three decades and (ii) a broader set of extreme but non-record events (p90–p99).

To link hydrometeorological extremeness with atmospheric drivers, we analyse the 1–96 h period preceding peak precipitation using 3-hourly CERRA reanalysis fields from 1000 to 100 hPa. Diagnostics include integrated water vapour (IWV), vertical humidity and water vapour profiles over peak-impact areas, absolute vorticity, and wind shear across multiple pressure-layer pairs.

Results show that the October 2024 event ranks as the most extreme autumn EPE in the record, with an unprecedented cumulative local magnitude of 4392 mm, nearly twice that of the second-ranked event (2275 mm in October 2000). The event is characterised by exceptionally high IWV values (~40 mm) over the affected region and a rapid IWV increase of approximately 0.4 mm h⁻¹ (around 25 mm in less than 72 h) prior to peak intensity. In addition, very strong vertical wind shear exceeding 25 m s⁻¹ between the surface and 400 hPa favoured sustained convective organisation and quasi-stationarity. Together, these results point to a compound thermodynamic–dynamic anomaly rather than a purely moisture- or dynamics-driven extreme. The proposed framework provides a physically consistent, basin-relevant benchmark for diagnosing exceptional Mediterranean flood-producing precipitation events using high-resolution observations and reanalysis-based process indicators.

How to cite: Espín, D., Benetó, P., and Khodayar, S.: The exceptional October 2024 flooding in Valencia (Spain): meteorological drivers of an extreme precipitation event, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19076, https://doi.org/10.5194/egusphere-egu26-19076, 2026.

EGU26-19395 | Orals | NP1.3

Heatwave response in quasi-equilibrium versus transient climate scenarios 

Susanna Corti, Claudia Simolo, Lea Rozenberg, Virna Meccia, and Federico Fabiano

Future changes in mean climate and extremes have been extensively assessed using model simulations of the 21st century under varying levels of anthropogenic greenhouse gas (GHG) forcing. Here, we examine the long-term climate legacy of an idealized abrupt stabilization of present-day and near-future GHG concentrations, with a focus on summer heatwaves across the Northern Hemisphere. Our analysis is based on multicentennial simulations performed with the EC-Earth3 model, in which external forcing is held fixed in time. After several centuries of internal adjustment, the climate system approaches a quasi-equilibrium state characterized by a stable level of global warming that depends strongly on the timing of forcing stabilization. Crucially, far-future quasi-equilibrium conditions can differ substantially from those that would arise if the same warming levels were reached by the end of the century, reflecting the distinct roles of fast and slow components of the Earth system. A key feature of the quasi-equilibrium response is a partial recovery of the Atlantic Meridional Overturning Circulation relative to transient simulations, which influences regional climate and leads to a pronounced amplification of heatwave frequency and intensity over the North Atlantic sector. Conversely, many land areas ultimately experience less severe heatwaves than in transient scenarios, owing to the slower warming rates in the stabilization experiments. Results show that the long-term response of extremes is shaped by the magnitude of global warming, as well as the pathway and timescale over which that warming is realized, highlighting the need for equilibrium-focused experiments in future climate risk assessments.

How to cite: Corti, S., Simolo, C., Rozenberg, L., Meccia, V., and Fabiano, F.: Heatwave response in quasi-equilibrium versus transient climate scenarios, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19395, https://doi.org/10.5194/egusphere-egu26-19395, 2026.

EGU26-19415 | ECS | Orals | NP1.3

Rareness Amplified INtensification of Extreme rainfall (RAINE): how the worst events get worse the fastest 

Iris de Vries, Frederic Castruccio, Dan Fu, and Paul O'Gorman

Floods associated with extreme precipitation cause tremendous damage and losses every year, and are projected to become more frequent and more severe with climate change in most land regions. Events of much higher intensities than previously observed can cause unforeseeably large impacts due to their unprecedentedness. The changing occurrence probability of such “surprise events” is closely related to changes in the statistical distribution of extreme precipitation: while a constant scaling with temperature (such as Clausius-Clapeyron) causes a constant fractional increase for all return levels, strong increases in the variability of extreme precipitation (distribution width) lead to relatively stronger intensification of the most extreme events. The latter change is indicative of increasing high-impact surprise event probabilities. Regions where rare extremes exhibit a faster relative intensification than moderate extremes (skewed intensification) are subject to RAINE: Rareness-Amplified INtensification of Extremes. In other words, RAINE means the worst events get worse the fastest.

We present a statistical framework based on extreme value theory to diagnose RAINE in annual maximum daily precipitation (Rx1d) from observations and simulations. We focus in particular on results from the 10-member high-resolution (0.25° atmosphere/land and 0.1° ocean) CESM1 ensemble (MESACLIP, historical+RCP8.5), which has been shown to simulate Rx1d quite accurately. We identify a strong RAINE-effect for most of the global land over the 21st century under RCP8.5. We categorise the data based on region and Rx1d-causing weather phenomenon, and find that a physical scaling based on vertical updraft and relative humidity explains the RAINE pattern. Different seasons, regions and phenomena feature different relative contributions of vertical updraft and relative humidity to RAINE, which can be linked to different environmental conditions and climate change effects governing Rx1d changes. In observations, robust distributional changes are difficult to detect due to high variability of extreme precipitation. Our combined statistical and physical characterisation of RAINE can help explain and constrain uncertainties in future risks posed by unprecedented extreme precipitation.

How to cite: de Vries, I., Castruccio, F., Fu, D., and O'Gorman, P.: Rareness Amplified INtensification of Extreme rainfall (RAINE): how the worst events get worse the fastest, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19415, https://doi.org/10.5194/egusphere-egu26-19415, 2026.

EGU26-19524 | Orals | NP1.3

Are we closing in on true ‘end-to-end’ attribution? 

Rupert Stuart-Smith

Two decades of climate change attribution research have shed light on the impacts of climate change occurring worldwide. The first wave of attribution research quantified climate change impacts on the intensity and probability of extreme weather events and slow-onset changes in glaciers and sea levels. Over the past decade, impact attribution studies have extended these methods to assess the attributable impacts of extreme events on agriculture, health, economic losses and biodiversity. Concurrently, source attribution research quantified individual emitters’ contributions to climate change impacts.

The emissions of individual actors cause climate change impacts. The approximately linear relationship between cumulative CO2 emissions and global temperature rise, combined with the fact that many climate change impacts become progressively worse with rising global temperatures, provides a conceptual basis for this claim. Steady progress towards being able to quantify individual emitters’ contributions to specific losses has brought us closer to true ‘end-to-end’ attribution. However, while studies have quantified emitters’ contributions to aggregate impacts such as regional economic losses, are there circumstances in which we might be able to attribute specific, individual losses to individual actors? This presentation will discuss the scientific possibility of achieving this objective and the legal consequences that may follow.

How to cite: Stuart-Smith, R.: Are we closing in on true ‘end-to-end’ attribution?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19524, https://doi.org/10.5194/egusphere-egu26-19524, 2026.

EGU26-20508 | ECS | Orals | NP1.3

 Predicting extreme events by identifying precursors on the chaotic attractor manifold 

Kevin R. Schuurman, Richard P. Dwight, and Nguyen Anh Khoa Doan

Predicting spatiotemporal extreme events using dynamical systems theory poses several major challenges. One of these is the phase space dimensionality of spatiotemporal systems. Extreme events are rare, while the number of variables that could potentially drive them is large. Often, a subset of the phase space is sampled, or features are engineered based on previous research on drivers, to predict spatiotemporal extreme events. On the other hand, the background attractors are often assumed to be of much smaller dimensionality than the phase space. Therefore, we propose a novel framework that approximates the background attractor of chaotic systems using an autoencoder. On this lower-dimensional attractor representation, precursor densities are created from historical analogues. Based on these precursor densities, predictions of extreme events are made. This framework proves to be efficient in predicting extreme events in a simplified turbulent flow and a climate model. Without engineering-specific predictor feature sets, this lower-dimensional representation of the attractor allows for more efficient and accurate analog prediction of extreme events in large chaotic systems.

How to cite: Schuurman, K. R., Dwight, R. P., and Doan, N. A. K.:  Predicting extreme events by identifying precursors on the chaotic attractor manifold, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20508, https://doi.org/10.5194/egusphere-egu26-20508, 2026.

Climate change has impacts on natural systems and populations, which can be analysed in attribution studies and attempted to be predicted in forward-looking analyses. Climate extremes in particular can be very impactful, be it in in terms of extreme individual climate hazards, extreme combinations of climate hazards, or less extreme climatic conditions combined with particular settings of exposure and vulnerability resulting in severe impacts. As the field of impact attribution is burgeoning, different perspectives on these complexities become apparent in different study designs, with implications for the research questions they address and the potential role they might play beyond science.

Here, we will give an overview over different climate change impact approaches, including how they each do (or don’t) consider climate extremes. Besides different attribution framings and impact modelling approaches, we will present a discussion of the climate data types typically used in impact attribution, and their implication for capturing impacts of extreme weather and climate. We will especially talk about extreme event attribution framings, and how ‘event’ can be defined in different ways from climate and impact standpoints, respectively. The differences will be illustrated using references to existing literature as well as works in progress, particularly from the field of agriculture-related impacts on food security and nutrition-related health.

How to cite: Undorf, S.: Defining events and extremes in climate change impact attribution, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21133, https://doi.org/10.5194/egusphere-egu26-21133, 2026.

EGU26-21503 | ECS | Orals | NP1.3

Source attribution: From national emissions to global loss in working hours due to climate-change increased heat 

Paula Romanovska, Mark New, Christoph Gornott, Audrey Brouillet, and Sabine Undorf

Human-induced climate change has increased heat stress, leading to significant losses in work productivity and subsequent economic repercussions. Not only are the climate change-related losses in work productivity due to heat unequally distributed around the globe, but the contributions of individual nations to these losses through greenhouse gas emissions are also disproportionate. Here, we present a source attribution approach that links historical national emissions to global lost working hours resulting from increased heat exposure.

Following the framework of Callahan & Mankin (2022 & 2025), we conduct the source attribution study in three steps: First, we calculate the contribution of past national emissions to the change in global mean surface temperature (GMST) using the reduced-complexity climate model Finite amplitude Impulse Response (FaIR). Second, we apply a pattern scaling technique, trained on outputs from general circulation models, to translate GMST changes into grid-level heat stress metrics, here the wet bulb globe temperature (WBGT). Third, we use the simulated GMST changes due to national emissions, the pattern scaling coefficients, and two literature-based exposure-response functions to estimate the potential loss of working hours attributable to national emissions at grid level. By integrating demographic data on population and employment, we derive estimates of total potential losses in working hours linked to specific nations' emissions. Additionally, we thoroughly assess uncertainties arising from global climate models, the FaIR model, and the exposure-response functions.

Our preliminary results highlight the different responsibilities of nations for the costs associated with increased occupational heat stress. The study thereby contributes to the growing body of literature linking individual emitters with experienced harms, providing critical insight into climate liability and national accountability for climate policy.

 

Callahan, C. W., & Mankin, J. S. (2022). National attribution of historical climate damages. Climatic Change, 172(3–4), 1–19. https://doi.org/10.1007/S10584-022-03387-Y/FIGURES/4

Callahan, C. W., & Mankin, J. S. (2025). Carbon majors and the scientific case for climate liability. Nature 2025 640:8060, 640(8060), 893–901. https://doi.org/10.1038/s41586-025-08751-3

How to cite: Romanovska, P., New, M., Gornott, C., Brouillet, A., and Undorf, S.: Source attribution: From national emissions to global loss in working hours due to climate-change increased heat, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21503, https://doi.org/10.5194/egusphere-egu26-21503, 2026.

EGU26-21564 | ECS | Orals | NP1.3

Worst-Case European Heat and Drought Storylines generated using Ensemble Boosting 

Laura Suarez-Gutierrez, Urs Beyerle, Magdalena Mittermeier, Robert Vautard, and Erich M. Fischer

Heat and drought extremes pose escalating socio-economic and ecological risks, yet the most severe combinations of these high-impact extremes possible today remain poorly understood. Using thousands of plausible ensemble-boosting current climate storylines, we reveal the risk for more intense drought compounding with far more extreme heat and fire weather than ever experienced over Europe in the recent past. The most extreme boosted heatwaves surpass historical extremes in both intensity and particularly in persistence, and also exceed levels considered extreme in a 3°C warmer world by large margins. Some of the most extreme heatwaves arise under severe soil moisture depletion, while others develop under strong surface temperature gradients in the North Atlantic and extreme heat in the nearby Mediterranean and Atlantic basins, underscoring the diversity of pathways to worst-case conditions. Furthermore, our work reveals an additional risk: worst-case heatwaves occur predominantly after another extreme heatwave. This highlights the potential for aggravated impacts due to decreased recovery times and intensified heat stress on humans, ecosystems and infrastructure made more vulnerable by the first event. Given the scale, intensity, and unprecedented successive and compounding nature of these worst-case storylines, we underscore the urgent need for well-informed adaptation strategies that sufficiently reflect these risks. 

How to cite: Suarez-Gutierrez, L., Beyerle, U., Mittermeier, M., Vautard, R., and Fischer, E. M.: Worst-Case European Heat and Drought Storylines generated using Ensemble Boosting, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21564, https://doi.org/10.5194/egusphere-egu26-21564, 2026.

EGU26-22751 | Orals | NP1.3

Scaling of Rainfall Intensity and Frequency with Rising Temperatures 

Jun Yin, Bei Gao, and Amilcare Porporato

Global warming is projected to intensify the hydrological cycle, amplifying risks to ecosystems and society. While extreme rainfall appears to exhibit stronger sensitivity to global warming compared to mean rainfall rates, a unifying physical mechanism​ capable of explaining this systematic divergence has remained elusive. Here, we integrate theory and data from a global network of nearly 50,000 rain-gauge stations to unravel the rainfall intensity and frequency response to rising temperatures. We show that the distributions of wet-day rainfall depth exhibit self-similar shapes across diverse geographical regions and time periods. Combined with the temperature response of rainfall frequency, this consistently links mean and extreme precipitation at both local and global scales. We find that the most probable change in rainfall intensity follows Clausius-Clapeyron (CC) scaling with variations shaped by a fundamental hydrological constraint. This behavior reflects a dynamic intensification of updrafts in space and time, which produces localized heavy precipitation events enhancing atmospheric moisture depletion and hydrologic losses through runoff and percolation. The resulting reduction in evaporative fluxes slows the replenishment of atmospheric moisture, giving rise to the observed trade-off between rainfall frequency and intensity. These robust scaling laws for rainfall shifts with temperature are essential for climate projection and adaptation planning.

How to cite: Yin, J., Gao, B., and Porporato, A.: Scaling of Rainfall Intensity and Frequency with Rising Temperatures, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22751, https://doi.org/10.5194/egusphere-egu26-22751, 2026.

EGU26-23150 | Posters on site | NP1.3

Attribution study of the 2023-2024 Drought on the South of Africa. 

Sarah Sparrow, Iago Perez-Fernandez, and Simon Tett
In 2023-2024 austral summer (Dec-Mar), an intense drought caused severe economical and human losses in the South of Africa, resulting in a loss of 1/3 of the total crop harvest. Here we report on a fairly standard attribution study for the drought of 2023/24 summer to assess if human influence increased the occurrence and intensity of droughts in the region. We used HadGEM-GA6 data to assess the likelihood of observing these events in scenarios with/without anthropogenic activity using 3 month Standardized Precipitation Evapotranspiration index (SPEI3) to quantify drought intensity. The sensitivity to region choice was explored using definitions of South of 20S, South of 15S, the region analyzed in the last World Weather Attribution report as well as individual countries. Simulations (with and without human activity) for the climatological period (1970-2010) as well as for 2023-2024 specifically were compared. The influence of the El Niño Southern Oscillation (ENSO) on SPEI3 and associated attribution statements was considered by compositing simulations by year into El Niño and La Niña phases. When using HadGEM simulations for the historical period (1970-2010), results showed that simulations with human activity showed lower SPEI values compared to natural simulations, hence implying that South African is drier compared to a natural scenario. Nonetheless the probability of drought is sensitive to the region chosen for the analysis, for example, for the south of 20S the probability of drought is mostly between 1.1 - 2 times more likely in simulations with human activity, whereas in the WWA area this probability rises to 5.9 - 16.9. By contrast, in HadGEM simulations with the prescribed conditions of 2023-2024, the probability of drought is much higher but also shows more uncertainty.
In addition, human activity strengthened the intensity and frequency of the dry periods set up by El Niño conditions in most countries located in the South of Africa, but the occurrence of droughts changes with the region. For example, in Zimbabwe, drought occurrence is 1.8 more likely in simulations with human influence during El Niño events, whereas in South Africa and Zambia the drought occurrence is 1.6 and 3.2 times more likely respectively whereas in Malawi it remains unchanged. In addition, when considering the prescribed conditions of 2023-2024 the probability of drought rises drastically for all countries.

How to cite: Sparrow, S., Perez-Fernandez, I., and Tett, S.: Attribution study of the 2023-2024 Drought on the South of Africa., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-23150, https://doi.org/10.5194/egusphere-egu26-23150, 2026.

EGU26-493 | ECS | Orals | CL3.2.4

Storyline-based climate attribution reveals strong intensification of 2018-2022 multi-year droughts in Europe 

Ray Kettaren, Antonio Sanchez-Benitez, Helge Goessling, Marylou Athanase, Rohini Kumar, Luis Samaniego, and Oldrich Rakovec

Prolonged summer droughts represent a significant and growing threat across Europe, as their persistence hinders hydrological recovery and severely impacts water resources, ecosystems, and agricultural systems under ongoing climatic warming. These extended dry periods can create soil-moisture deficits, ecological stress, and amplified heat extremes. Understanding the response of multi-year droughts to different warming levels is vital for shaping both adaptation and mitigation strategies.

In this study, we investigate the behaviour and severity of the 2018-2022 European multi-year soil moisture drought across a range of climate warming levels. We apply an innovative storyline attribution approach, which enables a physically consistent comparison of the same drought sequence under different climate conditions. Specifically, we utilise spectrally nudged AWI-CM-1-1-MR, constrained to follow observed synoptic-scale circulation from ERA5, to force the mesoscale Hydrologic Model (mHM). This modelling setup allows us to specifically isolate how anthropogenic warming modifies soil-moisture deficits, without altering the real-world atmospheric conditions that triggered the drought sequence.

Under the present-day climate conditions, the 2018-2022 drought produced a soil-moisture deficit of -44 (±11.8) km3, affecting 0.63 (±0.07) million km2 (11.5% of the study area). In the absence of anthropogenic climate change (pre-industrial climate conditions), the 2018-2022 multi-year event would have shown a soil moisture surplus nearly double the magnitude of present-day losses, with drought spatial extent only about one-third of current levels. Future warming levels further exacerbate these impacts. With warming of 2 K to 4 K, the losses increase from -82 (±6.6) to -256 (±7.1) km3, while drought extent expands from approximately 16% to 43%.

Overall, our results demonstrate that rising global temperatures substantially intensify multi-year droughts by both enlarging their spatial footprint and deepening hydrological deficits. As climate warming increases the likelihood that single-year droughts transition into persistent multi-year events, the findings emphasise the urgent need for effective climate mitigation and adaptation strategies across Europe. A full version of this work is currently under review in Earth’s Future; the preprint can be accessed at https://doi.org/10.22541/au.176220208.89936181/v1 . 

How to cite: Kettaren, R., Sanchez-Benitez, A., Goessling, H., Athanase, M., Kumar, R., Samaniego, L., and Rakovec, O.: Storyline-based climate attribution reveals strong intensification of 2018-2022 multi-year droughts in Europe, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-493, https://doi.org/10.5194/egusphere-egu26-493, 2026.

EGU26-505 | ECS | Orals | CL3.2.4

Climate archetypes of simultaneous global crop failures  

Tamara Happé, Raed Hamed, Weston Anderson, Chris Chapman, and Dim Coumou

Most of the world's food is produced in a handful of countries, the so-called breadbaskets of the world. Due to climate change, there is an increasing risk of crop failures, due to compounding hot and dry extremes. Furthermore, certain climate drivers – through  teleconnections – have shown to lead to simultaneous crop failures around the globe. This highlights the importance to understand which climate processes drive global crop yield variability. Here we show global crop yield failures (Maize, Soya, Wheat, Rice, and combined) are associated with La Nina-like sea surface temperature (SST) anomalies, using Archetype Analysis. The adverse crop-yield archetypes show simultaneous hot-dry-surface imprints across the world, highlighting these high risk crop failure scenarios are driven by climate extremes. Our results demonstrate the importance in understanding the climate drivers of global crop production, and highlights the deep uncertainty associated with a changing climate. The response of ENSO due to anthropogenic activities is not yet fully understood and climate models often inaccurately reproduce the observed La Nina trends. Thus the fact that our results indicate that simultaneous crop failures are linked to La Nina like SSTs, highlights the deep uncertainty we currently face regarding food security in the future. 

How to cite: Happé, T., Hamed, R., Anderson, W., Chapman, C., and Coumou, D.: Climate archetypes of simultaneous global crop failures , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-505, https://doi.org/10.5194/egusphere-egu26-505, 2026.

EGU26-537 | ECS | Orals | CL3.2.4

Linking Emissions from Fossil Fuel Megaprojects to Lifetime Climate Extremes Across Generations and Multi-Century Committed Change  

Amaury Laridon, Wim Thiery, Rosa Pietroiusti, Chris Smith, Joeri Rogelj, Jiayi Zhang, Carl-Friedrich Schleussner, Inga Menke, Harry Zekollari, Lilian Schuster, Alexander Nauels, Matthew Palmer, and Jacob Schewe

Carbon bombs comprise 425 fossil fuel megaprojects whose cumulative potential emissions exceed by at least a factor of two the remaining global carbon budget compatible with the Paris Agreement. The full exploitation of these projects would therefore generate substantial additional warming. As high-impact climate extremes intensify with each increment of warming, a central challenge is to quantify how emissions from individual projects translate into concrete physical and societal impacts across current and future generations. 

Within the Source2Suffering project, we develop a modelling framework that links project-level CO₂ and CH₄ emissions to lifetime exposure to six categories of high-impact climate extremes, including heatwaves, droughts, and floods, using a storyline-based approach. The framework also quantifies each project’s contribution to committed glacier mass loss and multi-century sea-level rise. By explicitly representing uncertainties, it provides probabilistic estimates of how warming increments induced by individual fossil fuel projects propagate through physical processes to generate compound and cascading risks. 

The results reveal marked spatial and intergenerational inequalities in exposure. These arise from (i) physical mechanisms that amplify extreme hazards in many regions of the Global South, and (ii) demographic trends that concentrate most of the world’s present and future population in these highly affected areas. By establishing a tractable link between specific emission sources, the physical drivers of high-impact extremes, and their long-term societal consequences, this framework contributes to the development of scientifically grounded information to support climate mitigation efforts. 

How to cite: Laridon, A., Thiery, W., Pietroiusti, R., Smith, C., Rogelj, J., Zhang, J., Schleussner, C.-F., Menke, I., Zekollari, H., Schuster, L., Nauels, A., Palmer, M., and Schewe, J.: Linking Emissions from Fossil Fuel Megaprojects to Lifetime Climate Extremes Across Generations and Multi-Century Committed Change , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-537, https://doi.org/10.5194/egusphere-egu26-537, 2026.

EGU26-1535 | ECS | Orals | CL3.2.4

Regional aerosol changes modulate the odds of record-breaking heat extremes 

Florian Kraulich, Peter Pfleiderer, and Sebastian Sippel

Record-breaking heat extremes imply large health risks and can disrupt critical infrastructure, because societies are often adapted only up to previously observed extremes. Understanding how new records evolve is therefore essential. The probability of record-breaking heat events depends on the regional warming rate. This rate is mainly driven by greenhouse gas-induced global warming and has increased in recent decades. The resulting annual probability of record-breaking heat extremes is additionally modified in a nonlinear way by other regional forcing changes, such as aerosols. Because aerosol concentrations have changed substantially in many regions, they can amplify or reduce the annual likelihood of exceeding previous temperature records. 

We first analyze single forcing large ensemble simulations that isolate the effects of aerosols and greenhouse gases. In Europe, decreasing aerosol concentrations have increased the regional warming rate and thereby the probability of record-breaking heat extremes by about 35% today. In contrast, in South Asia, where aerosol concentrations are increasing, we find a dampening of record-breaking probabilities of about 40%. To evaluate the effect of near-future aerosol reductions, we use simulations from the Regional Aerosol Model Intercomparison Project (RAMIP). In RAMIP, aerosol emissions are reduced from SSP3-7.0 to SSP1-2.6 either globally or only in selected regions. This allows us to analyze the regional effects of aerosol reductions as well as their remote responses. In general, aerosol reductions lead to an increased probability of record-breaking heat extremes.

Finally, we examine recent observed record-breaking events and evaluate whether their regional frequency matches the expected record breaking probabilities from model simulations. We expect that changes in aerosol concentrations contribute to changes in the annual record-breaking probability in regions with major aerosol concentration changes in recent decades, such as Europe, North America, East Asia, and South Asia. Overall, these results suggest that changes in aerosol concentrations are important for the present and near-future probability of record-breaking heat extremes.

How to cite: Kraulich, F., Pfleiderer, P., and Sippel, S.: Regional aerosol changes modulate the odds of record-breaking heat extremes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1535, https://doi.org/10.5194/egusphere-egu26-1535, 2026.

EGU26-2212 * | Orals | CL3.2.4 | Highlight

Challenges and Opportunities for Understanding Societal Impacts of Climate Extremes 

Gabriele Messori, Emily Boyd, Joakim Nivre, and Elena Raffetti

Climate extremes exact a heavy and differential toll on society. Reported economic losses are primarily concentrated in developed economies, whereas reported fatalities occur overwhelmingly in developing economies. Moreover, even at single locations the adverse impacts of extreme climate events are often unequally distributed across the population. Understanding such impacts holds enormous societal and economic value, and is a key step towards climate resilience and adaptation. Recent research advances include improved impact forecasting and enhanced understanding of how the interaction between human and natural systems shapes the impacts of climate extremes. Nonetheless, there are some key challenges that have hindered progress. We focus on three: Limited availability and quality of impact data, difficulties in understanding the processes leading to impacts and lack of reliable impact projections. We argue that newly released datasets and recent methodological and technical advances open a window of opportunity to address several dimensions of these challenges. Notable examples include extracting impact information from textual sources using large language models and developing impact projections using data-driven approaches. Moreover, interdisciplinary collaborations between the social and natural sciences can elucidate processes underlying past climate impacts and enable building storylines of future societal impacts. We call for building momentum in seizing these opportunities for a breakthrough in the study of impacts of climate extremes. Achieving meaningful progress will require interdisciplinary and intersectoral research, and strong collaboration across academic, policy and practitioner communities.

How to cite: Messori, G., Boyd, E., Nivre, J., and Raffetti, E.: Challenges and Opportunities for Understanding Societal Impacts of Climate Extremes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2212, https://doi.org/10.5194/egusphere-egu26-2212, 2026.

EGU26-2537 | ECS | Orals | CL3.2.4

Dry and moist convective upper bounds for extreme surface temperatures 

Quentin Nicolas and Belinda Hotz

How hot can heatwaves get in a given region of the world? The current pace of climate change challenges the statistical methods traditionally used to answer this question. An alternative approach is to seek a physics-based upper bound to extreme surface temperatures (Ts). Recent work proposed to address this problem using the hypothesis that convective instability limits the development of heat extremes. Here, we show that under this hypothesis, the absolute upper bound for extreme Ts --- obtained in the limit of zero surface humidity --- is set by dry convection: that is, this bound is reached when the mid-troposphere and the surface are connected by a dry adiabat. Previous work suggested that this upper bound is instead set by moist convective instability and is several degrees hotter. We resolve this discrepancy by showing that moist convection only limits heatwave development when surface specific humidity is larger than a threshold, and that the moist convective upper bound cannot exceed the dry limit. Yet, numerous temperature profiles in observational and reanalysis records do exceed the dry convective limit. We show that these occur exclusively in regions with an extremely deep boundary layer and where a daytime superadiabatic layer develops near the surface. We conclude with an overview of the different upper bounds applicable in dry and moist scenarios, including the roles of processes such as entrainment and convective inhibition.

How to cite: Nicolas, Q. and Hotz, B.: Dry and moist convective upper bounds for extreme surface temperatures, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2537, https://doi.org/10.5194/egusphere-egu26-2537, 2026.

EGU26-2749 | Posters on site | CL3.2.4

Co-occurrence of large hail and heatwaves in European regions in current and future climate scenarios 

Ellina Agayar, Brennan Killian, Iris Thurnherr, and Heini Wernli

Large hail and heatwaves are among the most extreme weather phenomena, posing serious risks to human health, ecosystems, and infrastructure, while also leading to significant economic losses. However, the co-occurrence of large hail and heatwaves, and the potential physical mechanisms linking these two phenomena, remain poorly understood. In this study, we investigate the climatology of large hail and the atmospheric drivers of large hail and heatwave co-occurrences across selected European regions, using an 11-year convection-permitting climate simulation with the COSMO regional climate model (2011–2021). In addition, we assess how these extremes may evolve under future climate conditions (+3°C global warming).

Results show increases in large hail frequency across Europe in a warmer climate. In central and eastern regions, the frequency rises approximately 20 %, whereas in the Alpine, Mediterranean, and Baltic regions it nearly doubles. Exceptions are France and Spain, where large-hail frequency declines by 26% and 33%, respectively. Also, there is a notable correlation between the occurrence of heatwaves and large hail across central and eastern Europe.  This relationship is less evident in southern Europe, due to large hail occurs mainly in autumn storms caused by large-scale disturbances. Additionally, large hail during heatwave days is forms in environments with higher median values of most-unstable convective available potential energy and 2 m temperature than large hail in the absence of heatwaves. A spatiotemporal analysis revealed that the days leading up to large hail events increasingly coincide with heatwave conditions. In the present climate, large hail is most often found within ~500 km of heatwave boundaries, both inside and outside them. The future climate scenario indicates a spatial shift of large hail events beyond the heatwave extent across all continental domains.

How to cite: Agayar, E., Killian, B., Thurnherr, I., and Wernli, H.: Co-occurrence of large hail and heatwaves in European regions in current and future climate scenarios, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2749, https://doi.org/10.5194/egusphere-egu26-2749, 2026.

EGU26-2967 | ECS | Posters on site | CL3.2.4

Separating dynamic and thermodynamic contributions in Mediterranean extreme precipitation (in a storyline approach) 

Cosimo Enrico Carniel, Reto Knutti, and Erich Fischer

Extreme precipitation in the Mediterranean basin emerges from a complex interaction between large-scale circulation, moisture transport and mesoscale dynamics, making the most damaging events difficult to sample in conventional climate simulations. This work presents a storyline-based framework to explore  very rare and  extreme rainfall under present and future climate conditions. 

We apply ensemble boosting to the fully coupled CESM2 model to generate alternative realizations of the most intense precipitation events affecting the Southern Alps and the Spanish Mediterranean coast. Starting from a 35 member parent ensemble of CESM2, these occurrences are identified and resimulated through boosted ensembles, resulting in a large sets of dynamically consistent trajectories that preserve the synoptic evolution of the original event while sampling its internal variability by perturbing the initial conditions. Comparisons with ERA5 reanalysis and available observations are performed to assess the realism of the simulated circulation patterns and precipitation characteristics associated with these extreme events. 

Preliminary results demonstrate that ensemble boosting successfully reproduces the temporal evolution of reference precipitation extremes, with many boosted members closely matching the timing and peak intensity of the parent events. In several cases, individual boosted realizations exceed the peak intensity of the reference simulation, revealing physically consistent more intense scenarios within the same large-scale setup. The amplification potential depends strongly on the perturbation lead time: short lead starts tend to cluster near the reference intensity, whereas longer lead times display a broader ensemble spread and occasionally generate substantially stronger or delayed rainfall peaks. 

In a second step, a conditional attribution methodology is applied in which the large-scale circulation is constrained while the thermodynamic background is modified to represent different climate states. This allows us to isolate the thermodynamic contribution of climate change to extreme precipitation intensity, providing physically interpretable estimates of how much more intense these events become in a warmer climate. 

By bridging weather-scale event evolution with climate-scale statistics, this approach provides new insight into the physical limits of Mediterranean extreme precipitation and offers a robust basis for assessing future extreme rainfall scenarios. 

How to cite: Carniel, C. E., Knutti, R., and Fischer, E.: Separating dynamic and thermodynamic contributions in Mediterranean extreme precipitation (in a storyline approach), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2967, https://doi.org/10.5194/egusphere-egu26-2967, 2026.

EGU26-3456 | ECS | Orals | CL3.2.4

Demonstrating the plausibility of worst-case month-long heatwave storylines in Western Europe 

Florian E. Roemer, Erich M. Fischer, Robin Noyelle, and Reto Knutti

What are the worst-case heatwaves that are plausible in the present or near-future climate? Model-based experiments using ensemble boosting, a computationally efficient method to simulate unprecedented extremes, suggest that month-long heatwaves that break previous records by more than 5 K across Germany and France are possible in the near future. But how can we assess the plausibility of these heatwaves unprecedented in the observational record? We here test whether the most extreme simulated month-long heatwaves in Germany and France are consistent with current process understanding and with historical heatwaves.
We show that despite their extreme record-breaking characteristics both events cannot be ruled out as implausible. To demonstrate this, we compare these two worst-case events with historical heatwaves in the reanalysis record. To this end, we calculate standardized anomalies relative to a time-evolving climatology of relevant physical variables such as temperature, 500 hPa geopotential, surface solar radiation, and soil moisture. We focus on two different worst-case events — one in Germany and one in France — which exhibit distinct characteristics and physical drivers. The event in Germany features extreme anomalies in most physical drivers, particularly those associated with land-atmosphere feedbacks, and features three short heatwaves in quick succession. In contrast, the event in France mostly features less extreme anomalies in these drivers and consists of one less intense but very persistent heatwave caused by anomalously weak zonal flow combined with above-average southerly winds. Using a multilinear statistical model and comparing with historical analogues, we show that the characteristics and physical drivers of both events are consistent with current process understanding and with historical events.

How to cite: Roemer, F. E., Fischer, E. M., Noyelle, R., and Knutti, R.: Demonstrating the plausibility of worst-case month-long heatwave storylines in Western Europe, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3456, https://doi.org/10.5194/egusphere-egu26-3456, 2026.

EGU26-3579 | ECS | Posters on site | CL3.2.4

ERA5-Based Validation of Thermodynamic Extreme Heatwave Drivers of the Paris region in CMIP6 simulations. 

Maeve Mayer, Sylvie Parey, Claire Petter, Soulivanh Thao, and Pascal Yiou

Previous studies have argued that the upper bound of temperature extremes in mid-latitude regions is reached by minimizing near-surface moisture during high low-tropospheric temperatures. Here, we revisit these theories for the Île-de-France region using the ERA5 reanalysis and show that the highest annual temperatures occur within the moist-to-expected range of the summer (June–August) near-surface humidity distribution. However, during the most extreme events, relative humidity is minimized as soil moisture approaches the wilting point and the atmospheric boundary layer deepens. Using the statistical distributions of these indicators and their temporal evolution in ERA5, we evaluate the representation of thermodynamic drivers in selected CMIP6 large ensembles. Finally, we apply a recently published revised framework of dry convective instability to estimate maximum attainable temperatures in both ERA5 and CMIP6, highlighting how climate change may modify heatwave dynamics in the Paris region.

How to cite: Mayer, M., Parey, S., Petter, C., Thao, S., and Yiou, P.: ERA5-Based Validation of Thermodynamic Extreme Heatwave Drivers of the Paris region in CMIP6 simulations., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3579, https://doi.org/10.5194/egusphere-egu26-3579, 2026.

EGU26-4070 | ECS | Orals | CL3.2.4

Enhancing impact monitoring by using computational text analyses 

Mariana Madruga de Brito, Jingxian Wang, Jan Sodoge, Ni Li, and Taís Maria Nunes Carvalho

Climate extremes, such as floods, heatwaves, and droughts, have myriad impacts across natural and social systems. However, traditional methods used for monitoring impacts tend to focus on single hazards or indicators (e.g., fatalities), address only quantitative consequences (e.g., economic losses), and frequently overlook indirect and social consequences (e.g., conflicts, mental health). Here, we show how text data can be used to measure the societal impacts of climate extremes across diverse text sources, including newspapers, social media, and Wikipedia articles.

First, we analyze over 26,000 newspaper articles on the July 2021 river floods in Germany to reveal cascading impacts across sectors like infrastructure, water quality, mental health, and tourism. Second, Twitter data from the 2022 drought in Italy is used to map public concern and perceived consequences, which align with observed socioeconomic indicators. Finally, we scale our analysis globally with Wikimpacts 1.0, a database of climate impacts extracted from 3,368 Wikipedia articles covering 2,928 events from 1034 to 2024, providing national and sub-national records of deaths, injuries, displacements, damaged buildings, and economic losses.

Together, these case studies illustrate the value of text-derived impact datasets for complementing traditional monitoring approaches. We also discuss the challenges of using such datasets, including representational biases, uneven temporal and spatial coverage, and differences in how impacts are reported. We conclude by discussing how the field can move towards shared standards and best practices, enabling more comparable and transparent use of text data for monitoring the impacts of climate extremes.

How to cite: Madruga de Brito, M., Wang, J., Sodoge, J., Li, N., and Nunes Carvalho, T. M.: Enhancing impact monitoring by using computational text analyses, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4070, https://doi.org/10.5194/egusphere-egu26-4070, 2026.

EGU26-4263 | ECS | Orals | CL3.2.4

Why was the 2023 jump in global temperature so extreme? 

Julius Mex, Christophe Cassou, Aglaé Jézéquel, Sandrine Bony, and Clara Deser

Global surface air temperature (GSAT) reached unprecedented heights in 2023. The record of year-to-year temperature increases was surpassed by a significant margin, especially in early boreal fall. We attribute the majority of this seasonal jump to the onset and maturing stages of the 2023 El Niño event. Using a process-based analysis of multiple observational datasets, we show that the uniqueness of the 2023 event can be largely related to the La Niña-like ocean-atmosphere background state upon which it developed.
This resulted in (1) a steep year-to-year increase of Sea Surface Temperature (SST), particularly in mean atmospheric subsidence regions, leading to extreme reduction of low-cloud-cover and giving rise to a record-breaking change in the radiative budget over the central and eastern Indo-Pacific; (2) anomalous sustained precipitation over climatological high SSTs in the Western Pacific, fueling unusual diabatic heating and an exceptionally early increase in tropical tropospheric temperature in boreal fall, ultimately influencing the GSAT jump with an additional contribution from the North Atlantic.
Our study improves the understanding of the interactions between interannual internally-driven processes and changes in mean climate background state, which a changing background is crucial to assess the evolution and modulation of anthropogenically-driven trends.

How to cite: Mex, J., Cassou, C., Jézéquel, A., Bony, S., and Deser, C.: Why was the 2023 jump in global temperature so extreme?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4263, https://doi.org/10.5194/egusphere-egu26-4263, 2026.

EGU26-4462 | ECS | Orals | CL3.2.4

Future cost of climate change for humanitarian crises 

Juha-Pekka Jäpölä, Anna Berlin, Charlotte Fabri, Arthur Hrast Essenfelder, Sepehr Marzi, Karmen Poljanšek, Michele Ronco, Steven Van Passel, and Sophie Van Schoubroeck

Humanitarian crises are the tip of the iceberg in climate change adaptation, yet their future is rarely quantified in human and economic terms. We use machine learning to simulate future estimates of people in need of humanitarian aid and required funding under the business-as-usual scenario (SSP2-RCP4.5) with warming of 2.1–2.4°C by 2100. Humanitarian needs rise to a baseline of 410±22 million people and USD2024 64±8 billion annually by 2050 worldwide, increases of 28% and 30% respectively compared to the current (320 million people and USD 49 billion). A lightly optimistic simulation holds needs near the current, while a medium pessimistic simulation leads to 614±68 million people and USD2024 96±19 billion by 2050, increases of 92% and 96% respectively. Our results show empirical vulnerabilities and an opportunity cost, as resources for crisis response displace funding for adaptation and mitigation. Yet, sustained investment could curb the impacts even with climate inertia.

How to cite: Jäpölä, J.-P., Berlin, A., Fabri, C., Hrast Essenfelder, A., Marzi, S., Poljanšek, K., Ronco, M., Van Passel, S., and Van Schoubroeck, S.: Future cost of climate change for humanitarian crises, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4462, https://doi.org/10.5194/egusphere-egu26-4462, 2026.

EGU26-4864 | ECS | Posters on site | CL3.2.4

Assessing the UNSEEN Flood-Relevant Winter Extreme Precipitation Over the Island of Ireland in the Present Climate 

Mohamed Bile, Conor Murphy, and Peter Thorne

Ireland’s winters are getting wetter, with more frequent heavy precipitation events increasing flooding risk across the Island. Extreme precipitation is a key driver of flooding in northwestern Europe; however, observational records are relatively short and represent only a single realisation of the climate state. As a result, they are inadequate for sampling low-likelihood, high-impact flood-relevant extreme precipitation events and for quantifying plausible maxima of such extremes. In this study, we quantify plausible maxima for flood-relevant winter precipitation under the current climate. We apply the UNprecedented Simulated Extremes using Ensembles (UNSEEN) approach to the flood-relevant winter precipitation indices (Rx1day, Rx5day, and Rx30days), using daily winter observations, the ECMWF SEAS5 seasonal prediction systems, and the CANARI Single Model Initial-condition Large Ensemble (SMILE) over the Island of Ireland. These indices are consistently derived across observations, pooled SEAS5 winter ensembles (ensemble member x lead times), and the CANARI SMILE. Model fidelity for CANARI and ensemble independence, stability, and fidelity for pooled SEAS5 are assessed to ensure that both models realistically represent extreme precipitation. Preliminary results indicate that both SEAS5 and the CANARI sample the physically plausible Rx1day and Rx5day extremes that exceed the maximum observed in the current climate, while neither system produces UNSEEN values exceeding the observed maximum Rx30day.  The CANARI large ensemble passes the fidelity test without bias correction, whereas the SEAS5 passes the fidelity test after applying simple multiplicative mean scaling bias correction. For CANARI, plausible maxima are approximately 18.01% higher for Rx1day and 20.77% higher for Rx5day than observed maxima, while Rx30day plausible maxima are approximately 8.70% lower than the highest observed Rx30day. For SEAS5, plausible maxima exceed observations by approximately 3.05% for Rx1day and 17.68% for Rx5day, while Rx30day plausible maxima are approximately 17.74% lower than the highest observed. These results highlight the limitations of observational records in sampling extreme tails and indicate that CANARI SMILE captures a broader range of internal climate variability than the initialised SEAS5 seasonal prediction system. They also show that UNSEEN ensembles are more effective at sampling short-duration precipitation extremes (Rx1day and Rx5day) than longer-duration accumulation precipitation extremes (Rx30day). Our study highlights the value of combining the UNSEEN approach with both seasonal prediction systems and SMILEs to better understand unprecedented flood-relevant precipitation extremes in the current climate.

How to cite: Bile, M., Murphy, C., and Thorne, P.: Assessing the UNSEEN Flood-Relevant Winter Extreme Precipitation Over the Island of Ireland in the Present Climate, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4864, https://doi.org/10.5194/egusphere-egu26-4864, 2026.

Many countries rely on international trade to ensure food security. With climate change and projected increases in the frequency and severity of extreme weather events, a significant portion of currently traded crops is vulnerable to climate extremes. While many studies have quantified the impact of extreme weather on crop production, few have linked these impacts to international trade and analyzed how future risks differ from the past. In this study, I combined crop modeling with FAOSTAT on crop and food trade data to identify the worst-case scenario in which extreme weather affects global staple crop trade. Six staple crops were included in the analysis. Probability distributions of each crop’s production were estimated for both historical and future periods under the 2020 crop distribution baseline. The worst-case scenario was determined based on the amount of traded crop affected in the past and future climates. The results provide insight into how future risks differ from historical patterns and whether international trade can continue to ensure food security under changing climate conditions.

How to cite: Su, H.: Identify the worst-case scenario where extreme weather has the greatest impact on the global staple crop trade, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5916, https://doi.org/10.5194/egusphere-egu26-5916, 2026.

EGU26-8004 | ECS | Posters on site | CL3.2.4

Better serving impact assessments via AI: Reconstructing daily extremes from spatiotemporal downscaling of monthly fields 

Yu Huang, Sebastian Bathiany, Shangshang Yang, Michael Aich, Philipp Hess, and Niklas Boers

Climate impact assessment studies strongly depend on fine representations of meteorological fields. Downscaling addresses the trade-off between data requirements and storage capacity, yet the faithful replication of extreme-value statistics and spatiotemporal consistency presents a persistent issue. We present an efficient generative AI model for spatiotemporal downscaling. Using coarse-resolution monthly fields as inputs, the model reconstructs sequences of daily fields with the enhanced spatial resolution. The AI-generated daily fields accurately reproduce spatial coherence, temporal persistence, and extreme-value characteristics, showing strong agreement with ground-truth daily observations. We look forward to applying this framework more effectively to future studies on the impacts of extreme events. 

How to cite: Huang, Y., Bathiany, S., Yang, S., Aich, M., Hess, P., and Boers, N.: Better serving impact assessments via AI: Reconstructing daily extremes from spatiotemporal downscaling of monthly fields, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8004, https://doi.org/10.5194/egusphere-egu26-8004, 2026.

EGU26-8241 | ECS | Posters on site | CL3.2.4

A process-based physical climate storyline for the Hercules storm in Portugal: extreme coastal flooding under climate change 

Gil Lemos, Pedro MM Soares, Ricardo Simões, Carlos Antunes, Ivana Bosnic, and Celso Pinto

In the beginning of 2014, exceptionally energetic swells associated with the Hercules storm (also known as “Christina”) produced one of the most devastating coastal events ever recorded in Portugal. Between January 6th and 7th, coastal flooding affected more than 30 municipalities along the Portuguese coastline, with offshore buoys registering maximum individual wave heights and periods of 14.91 m and 28.10 s, respectively. The storm resulted in more than 16 million euros in direct damages due to overtopping and coastal flooding, while indirect losses (considering affected businesses and populations) are estimated to have reached hundreds of millions of euros. In this study, two physical climate storylines are developed to assess the impacts of a “Hercules”-like storm, at five key-locations along the Portuguese coastline, occurring by the end of the 21st century, under the combined influence of sea-level rise (SLR), projected changes in wave climate, and altered coastal morphology, while retaining the same statistical representativeness observed in 2014. The storyline approach enables a clear linkage to the original event and facilitates the assessment of future extreme events such as Hercules within the context of a changing climate, supporting decision-making by working backwards from specific vulnerabilities or decision points. Results indicate that the impacts of a future Hercules-like storm are projected to intensify, considering SLR and increases in high-percentile wave energy. Extreme coastal flooding is expected to affect 1.9 to 2.4 times more area than in 2014, resulting in 3.2 to 6.5 times more physically impacted buildings, particularly in densely urbanized coastal sectors. As coastal erosion is expected to reduce the natural protection of Portuguese sandy coastlines, the currently employed protection mechanisms will require robust adaptation measures, strategically defined to withstand long-return-period extreme events.

 

This work is supported by FCT, I.P./MCTES through national funds (PIDDAC): LA/P/0068/2020 - https://doi.org/10.54499/LA/P/0068/2020, UID/50019/2025, https://doi.org /10.54499/UID/PRR/50019/2025, UID/PRR2/50019/2025. The authors would like also to acknowledge the project “Elaboração do Plano Municipal de Ação Climática de Barcelos (PMACB).

How to cite: Lemos, G., MM Soares, P., Simões, R., Antunes, C., Bosnic, I., and Pinto, C.: A process-based physical climate storyline for the Hercules storm in Portugal: extreme coastal flooding under climate change, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8241, https://doi.org/10.5194/egusphere-egu26-8241, 2026.

EGU26-9101 | Posters on site | CL3.2.4

Hot-dry compound events in the European Alps: Multi-century assessment (1600-2099 CE) indicates the need for fast adaptation 

Raphael Neukom, Tito Arosio, Alessandra Bottero, Anne Kempel, Veruska Muccione, Christian Rixen, Kerstin Treydte, and Pierluigi Calanca

Compound hot–dry events have recently led to severe consequences globally, often triggering cascading impacts across ecological and socio-economic systems. Currently, most analyses of hot–dry extremes rely on short observational records or projections, limiting evaluation against pre-industrial variability—the climatic range to which many natural and human systems adapted over centuries. This makes it difficult to place impacts of the increased intensity and frequency of compound events in an appropriate context for examining adaptation needs.

Here we leverage a unique data coverage in the Swiss Alps to quantify changes in summer mean climate and in compound hot–dry extremes and their associated return periods from 1600 to 2099 CE. Data used include multi-century temperature and atmospheric drought reconstructions from tree rings going back to 1600 CE, instrumental station records, and local-scale climate projections for 1981-2099.

Copula-based modelling shows that summers classified as extreme in pre-industrial conditions have become common in today's climate and are expected to correspond to cold and wet conditions by the end of the century. Our analysis further shows that the hot–dry conditions witnessed in summer 2003—characterized by simultaneous positive temperature and vapor pressure deficit (VPD) anomalies of 5.3°C and 2.6 hPa relative to the pre-industrial mean, respectively—were unprecedented over at least the past 400 years and are projected to remain rare until the end of the century under RCP2.6. By contrast, they are likely to occur every 2-3 years under RCP4.5 and even to become colder and wetter than average by 2070-2099 under RCP8.5, since in the latter case, temperature and VPD anomalies are projected to exceed pre-industrial conditions by 10.4°C and 8.1 hPa in the extreme case (30-year return period).

Without countermeasures, the consequences of these changes will include, among other things, dramatic losses in agricultural production and undesirable changes in forest ecosystem dynamics. Ultimately, our analysis suggests that rapid adaptation is necessary to avoid facing more frequent extreme heat and drought conditions than those observed under pre-industrial conditions. Under RCP8.5, in particular, socio-ecological systems will need to continuously adapt within 15 years to changes in the average climate to avoid facing high-impact hot-dry compound event frequencies higher than those experienced at any time over the past 400 years. Given that adaptation in mountain regions is currently not keeping up with the realized and projected climate impacts, as pointed out in several studies, we argue that the required speed of adaptation can pose substantial challenges for alpine societies.

How to cite: Neukom, R., Arosio, T., Bottero, A., Kempel, A., Muccione, V., Rixen, C., Treydte, K., and Calanca, P.: Hot-dry compound events in the European Alps: Multi-century assessment (1600-2099 CE) indicates the need for fast adaptation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9101, https://doi.org/10.5194/egusphere-egu26-9101, 2026.

EGU26-9800 | ECS | Posters on site | CL3.2.4

Sensitivity of Storm Boris rainfall intensification to wind nudging strength in event-based climate-change storyline simulations 

Antonio Sánchez Benítez, Marylou Athanase, and Helge F. Goessling

Understanding how climate change influences environmental extremes is vital for developing effective adaptation and mitigation strategies. In this study, we apply an event-based storyline approach to assess changes in accumulated precipitation associated with Storm Boris, which impacted Central Europe in September 2024. We examine both historical changes (attribution) and future projections and extend previous work by investigating the sensitivity of results to the degree of imposed dynamical constraint. Using the global CMIP6 coupled climate model AWI-CM1, we nudge simulations toward observed ERA5 winds—including the jet stream—across a range of climate backgrounds: preindustrial, present-day, and possible future states with 2, 3, and 4 °C global warming relative to preindustrial conditions. Two nudging configurations are compared: (1) a “weak constraint” configuration, in which only synoptic- and planetary-scale winds in the free troposphere are nudged, permitting some dynamical adjustment with warming; and (2) a “strong constraint” configuration, in which winds at all vertical levels and scales are imposed, thereby completely suppressing dynamical changes.

Both configurations capture the event, with stronger present-day rainfall in the strongly constrained configuration. The observed climate change between pre-industrial and present day is robust, with increases of 7% (4%) in accumulated rainfall under the weak (strong) constraint. Projections up to a 3ºC warmer climate show linear increases in the accumulated rainfall for both configurations. Beyond +3ºC, the response strongly diverges. Under weak constraint, rainfall changes at +4ºC are marginal or even mildly reduced relative to present-day, whereas the strongly constrained configuration continues to show linear increases. This divergence is linked to thermally-driven dynamical adjustments permitted under weak constraint. Whether these adjustments reflect a realistic response or methodological artifacts, and whether similar behaviour occurs in other events, remains to be explored. Our results highlight remaining uncertainties in storyline-based extreme precipitation projections, and demonstrate the importance of considering multiple possibilities.

How to cite: Sánchez Benítez, A., Athanase, M., and Goessling, H. F.: Sensitivity of Storm Boris rainfall intensification to wind nudging strength in event-based climate-change storyline simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9800, https://doi.org/10.5194/egusphere-egu26-9800, 2026.

EGU26-10410 | ECS | Orals | CL3.2.4

Extreme rainfall attribution distorted by structural warming biases in climate models 

Damián Insua Costa, Marc Lemus Cánovas, Martín Senande Rivera, Victoria M. H. Deman, João L. Geirinhas, and Diego G. Miralles

While the performance of climate models in simulating the magnitude of global warming has been extensively assessed, their fidelity in representing the three-dimensional (3-D) structure of warming, and how this affects extreme event attribution, remains poorly understood. Pseudo-global-warming experiments implicitly assume that imposed anthropogenic warming perturbations realistically capture the observed vertical and horizontal distribution of atmospheric temperature change. However, this assumption is rarely evaluated explicitly.

We diagnose 3-D structural warming discrepancies by comparing a representative set of six CMIP6 climate models against ERA5 temperature trends over 1940–2024. We show that widely used models exhibit systematic vertical and horizontal warming biases, typically over-amplifying warming in the mid-to-upper troposphere while damping the response near the surface, particularly across Northern Hemisphere mid-latitudes. We further show that these structural biases propagate into substantially different estimates of extreme rainfall intensification.

Using an ensemble of 81 high-resolution MPAS simulations within a storyline attribution framework, we analyze the October 2024 Valencia flood-producing storm as a high-impact case study. The diagnosed anthropogenic rainfall signal is highly sensitive to the 3-D structure of the imposed warming: CMIP6-based counterfactual experiments yield weak reductions in extreme rainfall (~10%), whereas observation-constrained warming profiles produce a stronger and more significant anthropogenic contribution (~30%). This amplification arises from enhanced low-level moistening and increased convective instability, together with dynamically consistent upper-level flow strengthening. The results confirm that 3-D warming structure is a first-order control on extreme-rainfall attribution, and that persistent model-structural errors can lead to a systematic underestimation of attribution signals in mid-latitude, high-impact precipitation extremes.

How to cite: Insua Costa, D., Lemus Cánovas, M., Senande Rivera, M., M. H. Deman, V., L. Geirinhas, J., and G. Miralles, D.: Extreme rainfall attribution distorted by structural warming biases in climate models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10410, https://doi.org/10.5194/egusphere-egu26-10410, 2026.

EGU26-10755 | ECS | Posters on site | CL3.2.4

Ensemble boosting of extreme precipitation in the Alps 

Laurenz Roither, Andreas F. Prein, Erich Fischer, and Neil Aellen

The Alps, with their complex topography, important geographic location and varying climatic influences have become a highly vulnerable region. Especially extreme precipitation and its associated impacts - from floods to landslides - are directly amplified by this distinct local environment.

Because observational timeseries are rather short and sample only limited locations, the impact-producing extreme tail of the precipitation distribution remains largely unexplored. In addition, the non-stationarity of the climate system makes data from a past climate less useful for gaining insights into current and future conditions. Coarse resolution global climate models can be used to produce long simulations including rare extreme events, but important processes such as topographic forcing and deep convection are poorly resolved, which limits physical interpretability. A different approach is needed to produce robust and actionable climate information on the local scales required for stress testing, early warning, adaptation and risk mitigation.

We suggest expanding the method of Ensemble Boosting into the realm of high-resolution modeling. We employ a global ICON setup with 10-20 km grid spacing with a two-way nested kilometer-scale European domain. Our initial goal is to simulate the 2013 Northern Alps flooding using ERA5 initial conditions. We asses lead time sensitivities for reinitializing simulations to optimize for variability and intensity within the boosted ensemble. We expect to produce physically consistent, interpretable and realistic storylines based on a historic extreme precipitation event in the Alps. These storylines enable us to assess driving processes and test physical limits of extreme precipitation in today’s climatic conditions.

With the current focus on a specific region and event we want to exercise a proof of concept embedded in a user-oriented framework. Next steps include producing a catalogue of extremes sampling across event types with the goal to physically constrain the extreme tail of precipitation distributions to reduce uncertainty in extreme value estimation, and to estimate return periods. Further applications of our approach could also be focused on climate projections or pseudo global warming simulations to gain insights into possible extremes in future climates.

How to cite: Roither, L., Prein, A. F., Fischer, E., and Aellen, N.: Ensemble boosting of extreme precipitation in the Alps, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10755, https://doi.org/10.5194/egusphere-egu26-10755, 2026.

This study investigates the impact of climate change on the extreme 2020 Meiyu over the middle and lower reaches of the Yangtze River (MLYR) through global variable-resolution ensemble subseasonal hindcasts. Results reveal that post-1980 climate change enhanced the 2020 extreme Meiyu rainfall over the MLYR region by approximately 17.19% at monthly scale, while simultaneously decreasing light and moderate precipitation frequency but intensifying heavy and extreme precipitation occurrences. Climate change intensified the low-pressure over northern China and southern China while weakening the Western Pacific subtropical high and the low-pressure over the Indian Peninsula. The circulation pattern results in significant shear between northeasterly and northwesterly winds in the southern MLYR region, contrasting with the high-pressure dominance in the northern MLYR region. This configuration suppressed convergence, vertical motion, and precipitation in the northern MLYR while enhancing these processes along its southern. Comparison between frequently re-initialized and subseasonal simulations further demonstrates that subseasonal simulations, by allowing full development of interactions between regional systems and large-scale circulation, more realistically represent climate change impacts on Meiyu season. In contrast, the frequently updated initial conditions in re-initialized simulations constrain such feedback processes. This study highlights the importance of utilizing global variable-resolution simulations at subseasonal-scale for climate attribution studies. Future studies would benefit from improved subseasonal forecasting capabilities to enhance attribution reliability.

How to cite: Xu, M. and Zhao, C.: Investigating Climate Change Impacts on the 2020 extreme Meiyu Through Global Variable-Resolution Ensemble Subseasonal Hindcasts, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11244, https://doi.org/10.5194/egusphere-egu26-11244, 2026.

EGU26-11790 | Posters on site | CL3.2.4

Exploring the changing dynamics of atmospheric blocking with a modified event-based storyline approach 

Wenqin Zhuo, Antonio Sánchez-Benítez, Marylou Athanase, Thomas Jung, and Helge Gößling

How atmospheric circulation patterns associated with extreme weather respond to climate change remains a challenging question. To explore this issue, we combine spectral nudging in a global climate model (AWI-CM1) with hindcasts, similar to ensemble boosting, in an event-based storyline framework. We examine the dynamic response to climate change of selected atmospheric blocking events associated with winter cold-air outbreaks and summer heatwaves in Eurasia. First, the large-scale circulation during the preconditioning phase of a blocking is constrained by spectral nudging toward reanalysis data, ensuring that the synoptic and planetary-scale environment is realistically and consistently reproduced in different climate backgrounds. The nudging is then switched off a few days before the blocking onset, allowing the model (including the atmospheric circulation) to evolve freely. We generate an ensemble with perturbed initial conditions to sample internal variability of the blocking development due to chaotic error growth. By applying this procedure under pre-industrial and +4 °C warmer climates compared to the present-day climate, we can separate the thermodynamic effects of climate change from the dynamical response, and quantify how a warming climate modifies both the evolution of atmospheric blocking (e.g., intensity and persistence) and the associated extreme weather impacts. We find that the climate state exerts a moderate and event-specific influence on blocking dynamics.

How to cite: Zhuo, W., Sánchez-Benítez, A., Athanase, M., Jung, T., and Gößling, H.: Exploring the changing dynamics of atmospheric blocking with a modified event-based storyline approach, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11790, https://doi.org/10.5194/egusphere-egu26-11790, 2026.

EGU26-12438 | Orals | CL3.2.4

Surface flux contributions to Mediterranean heatwaves: a new Lagrangian diagnostic 

Vinita Deshmukh, Andreas Stohl, and Marina Dütsch

The increasing frequency of Mediterranean heatwaves is associated with widespread impacts on human health, agricultural productivity, and infrastructure. Previous studies have shown that large-scale circulation patterns, such as persistent ridges and atmospheric blocking, play a key role in triggering heatwaves, along with subsidence and warm-air advection. However, the intensity and persistence of these events depends not only on the advection of heat and moisture but also on the heat and moisture supplied by turbulent surface fluxes into the advected air mass. Sensible and latent heat fluxes modify air-mass temperature and humidity (and thus equivalent potential temperature) along transport pathways to the heatwave region. These flux contributions, and their relative importance for heatwave anomalies, remain uncertain.

In this study, the contribution of surface sensible and latent heat fluxes to near-surface moisture and temperature anomalies during heatwaves is quantified using a new Lagrangian framework that combines backward air-mass trajectories from the FLEXPART particle dispersion model with surface fluxes from ERA5 reanalysis data. Surface flux contributions to the moist static energy are estimated by coupling them with near-surface residence times of air parcels arriving in the heatwave region. The approach is first validated by showing that moist static energy at the heatwave location can be reproduced by the sum of the particle initial conditions (i.e., most static energy at trajectory termination points) and the surface flux contributions accumulated over the Lagrangian tracking period. Following this validation, surface flux contributions can be split into latent and sensible heat flux contributions and mapped geographically.

The method is then applied to two recent Mediterranean heatwaves to assess the relative roles of sensible and latent heat fluxes and to identify the dominant land and sea source regions. Overall, this framework provides a direct and physically consistent way to attribute the moist static energy associated with heatwaves to surface fluxes, offering new insights into the processes that build and maintain Mediterranean heatwaves.

How to cite: Deshmukh, V., Stohl, A., and Dütsch, M.: Surface flux contributions to Mediterranean heatwaves: a new Lagrangian diagnostic, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12438, https://doi.org/10.5194/egusphere-egu26-12438, 2026.

EGU26-12593 | ECS | Posters on site | CL3.2.4

Unprecedented storm surges across European coastlines 

Irene Benito Lazaro, Philip J. Ward, Jeroen C. J. H. Aerts, Dirk Eilander, and Sanne Muis

Recent research has considerably advanced our ability to model extreme storm surges. Nevertheless, simulating unprecedented events remains a challenge. Current large-scale storm surge studies often rely on conventional statistical approaches to extrapolate data beyond historical records. However, these approaches entail large uncertainties and lack the capacity to physically characterise individual events. Furthermore, research on unprecedented events primarily focuses on hazard magnitude, often overlooking other dimensions relevant for risk management decisions.

This study addresses these gaps by examining unprecedented storm surges at a European scale across multiple dimensions. We follow a large-ensemble approach to generate numerous alternative pathways of reality, capturing a broader range of climate variability than the observational records. By pooling ensembles from the ECMWF SEAS5 seasonal forecast and forcing the Global Tide and Surge Model (GTSM), we obtain a 525-year dataset of unbiased, independent storm surge events. This synthetic dataset enables the identification of physically plausible events beyond those found in historical records. We evaluate the dataset against reanalysis-based storm surges to uncover and characterise unprecedented events across three dimensions: magnitude, spatial extent and temporal occurrence. Understanding these different dimensions of unprecedence provides a significant advance in our knowledge of coastal flood risk in Europe and supports improved coastal flood risk management decisions.

How to cite: Benito Lazaro, I., Ward, P. J., Aerts, J. C. J. H., Eilander, D., and Muis, S.: Unprecedented storm surges across European coastlines, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12593, https://doi.org/10.5194/egusphere-egu26-12593, 2026.

EGU26-12603 | ECS | Posters on site | CL3.2.4

The influence of sea surface temperatures on moisture sources of Central European Storm Boris in September 2024 

Philipp Maier, Marina Dütsch, Imran Nadeem, Martina Messmer, and Herbert Formayer

This study investigates the role of climate-change-driven sea surface temperature (SST) anomalies in intensifying extreme precipitation associated with Storm Boris. During the period 12th to 16th September 2024, Storm Boris produced extreme precipitation and subsequent flooding in Central Europe, recording over 350 mm accumulated precipitation in five days in parts of Austria. To assess the influence of climate-change-driven SSTs in the Atlantic, Mediterranean and Black Sea, we perform pseudo experiments, in which the SSTs of these water bodies are systematically reduced by 2 K. For that purpose, a model chain consisting of the Weather Research and Forecasting (WRF) model coupled to the Lagrangian particle dispersion model FLEXPART run with back-trajectory settings and a moisture source and transport diagnostic is utilized. The WRF model is further run with wind and pressure nudging over the entire simulation period and without nudging during the event in order to separate thermodynamic and dynamic responses. The moisture uptakes and losses of air parcels arriving in the Central European study region are traced backward in time for up to ten days, enabling the identification of the dominant moisture sources contributing to the observed extreme precipitation. Our analysis reveals the Eastern Europe land areas and the Mediterranean – where SSTs exhibited a strong positive anomaly compared to the long-term climatology – as primary moisture sources for Storm Boris. We further show that the decrease in available moisture by SST reduction in the Black Sea and/or the Atlantic is partially compensated by additional moisture uptake in the Mediterranean. Finally, we assess the thermodynamic sensitivity of mean precipitation to SST changes by comparing the simulated rainfall across different historical SST climatologies. The results indicate an average precipitation increase of approximately 3 % per Kelvin of SST warming for this event, emphasizing the contribution of climate-driven SST increases to the extreme precipitation observed during Storm Boris.

How to cite: Maier, P., Dütsch, M., Nadeem, I., Messmer, M., and Formayer, H.: The influence of sea surface temperatures on moisture sources of Central European Storm Boris in September 2024, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12603, https://doi.org/10.5194/egusphere-egu26-12603, 2026.

EGU26-12831 | ECS | Posters on site | CL3.2.4

Towards actionable storylines: development of a reproducible workflow 

Niels Carlier

Storylines, or tales of future weather, are an increasingly popular climate communication strategy. Storyline research aims to inform about how extreme events arise and how severe they may become under different background climates, connecting scientific knowledge and lived experience. Central to this approach is a focus on plausibility rather than probability.  Such "what-if" scenarios can stress-test policy and infrastructure, guiding or strengthening adaptation efforts. This study presents a reproducible chain of methodological steps for constructing such tales through data mining, which is demonstratively applied to the EURO-CORDEX ensemble to produce a coherent and communicable extreme heat storyline for Belgium. We present the results from a first workshop with city officials and emergency coordinators, which successfully launched an ongoing dialogue between stakeholders and scientists about the broader use of storylines as an accessible tool for climate adaptation.

How to cite: Carlier, N.: Towards actionable storylines: development of a reproducible workflow, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12831, https://doi.org/10.5194/egusphere-egu26-12831, 2026.

EGU26-12895 | Orals | CL3.2.4

How reliably can we estimate trends of surface weather extremes? A conceptual study using ERA5 reanalyses 

Heini Wernli, Tomasz Sternal, Sven Voigt, Michael Sprenger, and Torsten Hoefler

How the frequency and intensity of extreme weather events is affected by global warming in different regions is one of the central questions of climate change research, with obvious direct implications for climate change adaptation. A standard approach of defining weather extremes is to consider the exceedance of a percentile threshold, calculated from the statistical distribution of a meteorological variable of interest in a predefined reference period. Trends can then be assessed by considering the frequency of threshold exceedances in a period that extends beyond the reference period. While this approach appears rather straightforward, it comes with several choices related to the parameter, percentile threshold, aggregation period, reference period, and boosting interval. Here aggregation period refers to the question whether, e.g., precipitation extremes are considered with a duration of 1 hour or 1 day or multiple days, and the boosting interval is the symmetric time window used to calculate percentiles for a given day of year. When checking these partly methodological choices in previous studies, e.g., those referenced in the IPCC report, it becomes evident that different studies made different choices. Since there is no obvious “best choice”, it is important to quantify the influence of these choices on the resulting trend estimates. Therefore, this study uses ERA5 reanalysis data to systematically and globally explore the trends in 2-m temperature (T2m) and precipitation (P) and their robustness with respect to the aforementioned parameters. Key results are that (i) trends vary strongly between regions, (ii) they are methodologically more robust for T2m than for P, (iii) in regions with weak P trends, the sign of the trend depends on the methodological choices. These explorative analyses with ERA5 data are complemented by synthetic data experiments, in particular to investigate the influence of the boosting window. We suggest that trend analyses of percentile threshold exceedances of any parameter in any dataset should consider these methodological sensitivities in order to communicate robust estimates.

How to cite: Wernli, H., Sternal, T., Voigt, S., Sprenger, M., and Hoefler, T.: How reliably can we estimate trends of surface weather extremes? A conceptual study using ERA5 reanalyses, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12895, https://doi.org/10.5194/egusphere-egu26-12895, 2026.

EGU26-13076 | ECS | Orals | CL3.2.4

Global characterisation of the vertical temperature anomaly structure of heat extremes over land in ERA5 

Belinda Hotz, Heini Wernli, and Robin Noyelle

The formation of surface heat extremes is usually described in terms of surface processes and upper-level dynamics. However, their full vertical temperature profile contains additional essential information about the involved processes and dynamics. So far, it remains unclear whether heat extremes are associated with characteristic vertical temperature anomaly profiles and how they vary across the globe.
In this study, we globally and systematically classify vertical temperature anomaly profiles during annual maximum 2-m temperatures, so-called TXx events, using a k-means clustering approach. After a suitable normalisation and scaling of the anomaly profiles, we find three clusters, whose global distribution closely follows the polar, mid-latitude, and tropical climate zones. The three clusters capture key structural differences of heat extremes. Within the tropical cluster, positive temperature anomalies during TXx events are confined to the (often deep) boundary layer and intensify progressively in the days leading up to the event, while the upper troposphere is not deviating from its climatological mean. The mid-latitude cluster also exhibits bottom-heavy temperature anomalies, which, however, extend throughout the full troposphere, showing a strong vertical coupling during heat extremes. In the polar cluster, heat extremes are characterised by deep tropospheric warm anomalies, accompanied by the erosion of the near-surface inversion layer, resulting in a shallow layer of particularly strong temperature anomalies near the ground.
These results show that while multiple physical mechanisms can generate a heat extreme, at first order, temperature anomaly profiles during heat extremes are very similar to each other within a given climate zone. The variability between TXx events is much larger than the variability between the median profile of different grid points in the same cluster. Besides, the temperature profiles of the most extreme events are more similar to those of their cluster than the more moderate events, suggesting a typical dynamics of the most extreme heat events. 

How to cite: Hotz, B., Wernli, H., and Noyelle, R.: Global characterisation of the vertical temperature anomaly structure of heat extremes over land in ERA5, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13076, https://doi.org/10.5194/egusphere-egu26-13076, 2026.

EGU26-13386 | Posters on site | CL3.2.4

An emergent constraint for the future frequency of European windstorms 

Matthew Priestley, David Stephenson, Adam Scaife, and Daniel Bannister

Windstorms are one of the most damaging natural hazards in western Europe, yet large inter-model spread limits robust assessment of future frequency changes. Previous assessments have suggested an increasing frequency, however models often have equal and opposite future responses. Using a novel statistical technique to quantify trends in these damaging windstorms we show that the historical mid-latitude meridional pressure gradient explains much of the inter-model variability in projected windstorm frequency across a large CMIP6 ensemble. Constraining projections using the pressure gradient index reduces uncertainty lowers the likelihood of increasing windstorm frequency and indicates a robust decline in pan-European windstorm frequency over the twenty-first century. We present a plausible mechanism via atmosphere–ocean feedbacks important for the North Atlantic storm track and circulation. These results suggest extreme increases in windstorm frequency are unlikely, despite projected increases in storm severity, with important implications for future loss and impact assessments.

How to cite: Priestley, M., Stephenson, D., Scaife, A., and Bannister, D.: An emergent constraint for the future frequency of European windstorms, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13386, https://doi.org/10.5194/egusphere-egu26-13386, 2026.

EGU26-13482 | ECS | Orals | CL3.2.4

Global projections of short-duration rainfall extremes using temperature-covariate models 

Jovan Blagojević, Andreas Prein, Nadav Peleg, and Peter Molnar

Short-duration, high-intensity rainfall extremes associated with convective storms pose a growing risk to urban areas under a warming climate, yet their future evolution remains difficult to quantify at the global scale using existing modelling approaches. Local projections are often constrained by the lack of long high-resolution observations and by the limited ability of climate models to accurately simulate sub-daily precipitation processes at the global scale. Here, we present a globally applicable framework for projecting changes in rare, short-duration rainfall extremes using temperature as a covariate in a non-stationary extreme value framework building on the TENAX model, driven entirely by global climate model output and without reliance on local observational data. The focus on rare, short-duration extremes directly targets the class of events responsible for a disproportionate share of climate-related impacts.


The approach links changes in rainfall intensity distributions to projected shifts in wet-day temperature distributions from CMIP6 models, integrating over the full temperature distribution rather than relying on uniform scaling or mean-shift assumptions. Dew-point temperature is employed as a proxy for atmospheric moisture availability, allowing thermodynamically constrained intensification of convective rainfall extremes to be represented consistently across climates. In an initial multi-regional application, the framework projects robust intensification of hourly-scale rare rainfall events, with increases of order 10–20% by late century under intermediate emissions scenarios and substantially larger changes under high-emissions pathways. Accounting for changes in the full temperature distribution shows that the strongest intensification occurs for the rarest events, which is underestimated when intensities are scaled only by mean temperature changes.


We further extend the framework to a global scale to assess spatial patterns and key structural uncertainties in projected short-duration rainfall intensification. Results highlight that methodological choices, including the selection of temperature covariate (dew-point versus surface air temperature), can introduce differences comparable to inter-model climate uncertainty in some regions, particularly in moisture-limited and continental climates. Treating these choices explicitly as structural uncertainties provides a clearer interpretation of projection robustness across diverse hydroclimatic regimes and highlights uncertainties beyond inter-model spread alone.


Overall, this work demonstrates that temperature-covariate approaches, when carefully formulated and driven by global climate models, offer a transferable and physically grounded pathway for projecting rare, short-duration rainfall extremes worldwide. The framework enables consistent global assessments in data-scarce regions and supports climate-change impact studies and urban adaptation planning by explicitly quantifying the uncertainties that matter most for short-duration rainfall risk.

How to cite: Blagojević, J., Prein, A., Peleg, N., and Molnar, P.: Global projections of short-duration rainfall extremes using temperature-covariate models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13482, https://doi.org/10.5194/egusphere-egu26-13482, 2026.

EGU26-13670 | Orals | CL3.2.4

Understanding, interpreting, and communicating future extreme precipitation risk using flow precursors 

Joshua Oldham-Dorrington, Camille Li, Stefan Sobolowski, Robin Guillaume-Castel, and Johannes Lutzmann

Many of the most societally impactful weather events in Europe occur on short timescales and there is a growing demand for improved projections of how such extremes will change in the future. That is, how will global climate change over decades impact extreme weather over days? The multiscale nature of this question challenges the capabilities of current earth system models, and this is especially the case for hydrometeorological extremes. Accurately simulating the hazards posed by extreme precipitation requires faithfully resolving interactions between the large-scale circulation, synoptic dynamics, the local boundary-layer, and hydrological and land surface conditions.

 

This is not only a quantitative modelling challenge, but a challenge of interpretation and narrative: the dynamics of extreme precipitation are diverse across space and time, and the statistics of the highest impact events are necessarily poorly constrained. These challenges are complicated further by the evergrowing size and hetereogeneity of multi-model datasets How can we explain model biases and trends in extreme precipitation? When models project similar changes in hydrometeorological risk do they do so for the same reasons? What implications do these factors have for regional downscaling and impact modelling? Can we relate future extremes quantitatively and robustly to historical high-impact events, as often requested by societal stakeholders?

 

We tackle these questions through a novel flow-precursor framework, applied to observational data, large ensemble climate simulations and subseasonal weather forecasts. We decompose extreme event risk into contributions from different scales and flow conditions, using regionally specific synoptic flow precursors which are directly associated with individual high-impact extremes or classes of extreme. These precursors are algorithmically identified and can be easily computed in large datasets, allowing us to obtain a physical interpretation of changing extreme risk across Europe without obscuring regional or seasonal diversity in precipitation dynamics.

 

We show how climate model biases and forced changes in extreme precipitation can be explained, categorised, and visualised in a succinct way that highlights important differences in their suitability for use in downscaling, impact modelling and storyline development. We demonstrate how dynamical decomposition can extract usable climate information even from heavily biased models, and how insights from models at different scales–such as from large climate ensembles and high-resolution weather forecasts–can be quantitatively synthesised to provide new insights on future hazards and plausible worst-case scenarios. Finally, we show how the method can be used to reframe complex, probabilistic climate projections and weather forecasts in terms of individual high impact historical events, aiding scenario visualisation, and allowing stakeholders to leverage their experience and domain knowledge when preparing for future high-impact extremes.

How to cite: Oldham-Dorrington, J., Li, C., Sobolowski, S., Guillaume-Castel, R., and Lutzmann, J.: Understanding, interpreting, and communicating future extreme precipitation risk using flow precursors, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13670, https://doi.org/10.5194/egusphere-egu26-13670, 2026.

EGU26-13840 * | ECS | Orals | CL3.2.4 | Highlight

Behind or ahead of committed warming: what it means for future hot extremes 

Dominik L. Schumacher, Victoria Bauer, Lei Gu, Lorenzo Pierini, and Sonia I. Seneviratne

Virtually all land regions have warmed over recent decades, yet heatwave trends show striking regional differences. The thermodynamic rise of hot extremes can be strongly modulated by atmospheric circulation, a phenomenon that has received increasing attention for regions such as Europe and parts of North America, where observed trends in hot extremes have been amplified and dampened, respectively. But what about other regions? How persistent are these circulation anomalies? And what are the implications for future heatwaves?

Using dedicated climate model experiments, we quantify how atmospheric internal variability has modulated historical heatwave trends globally. Building on a large ensemble framework, we interpret observed circulation contributions as placing regions on unusual warming trajectories — either well below or above the ensemble mean expectation. Regions currently displaying less warming compared to climate model simulations are effectively "lagging behind" the warming already committed to by anthropogenic forcing; those running warm are "ahead".

This warming trajectory position has profound implications for the pace of future change. Regions currently lagging behind, including much of North America, face substantially faster increases in hot extreme probability between now and the mid-century than ensemble mean projections suggest. Conversely, other regions have already experienced much of the expected probability increase. We illustrate these divergent futures through the evolving return period of what was once a 1-in-100-year hot extreme, showing how the present trajectory position determines the pace of change over the coming decades.

How to cite: Schumacher, D. L., Bauer, V., Gu, L., Pierini, L., and Seneviratne, S. I.: Behind or ahead of committed warming: what it means for future hot extremes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13840, https://doi.org/10.5194/egusphere-egu26-13840, 2026.

EGU26-14325 | ECS | Orals | CL3.2.4

A combined storyline-statistical approach for conditional attribution of climate extremes to global warming 

Dalena León-FonFay, Alexander Lemburg, Andreas H. Fink, Joaquim G. Pinto, and Frauke Feser

Quantifying the influence of anthropogenic global warming on extreme events requires both physical and statistical understanding. We present a framework combining two complementary conditional attribution methods: spectrally nudged storylines and flow-analogues. The storyline approach provides insights on how a specific event is shaped by the thermodynamic conditions representing past (counterfactual), present (factual) and future global warming levels (+2K, +3K, +4K). The flow-analogue method provides a statistical analysis of the recurrence of the observed event, and the future storyline-projected events based on similar dynamical patterns that lead to the event of interest. Together, this combined approach allows us to determine not only the change in likelihood of an extreme event occurring as it did in the present, but also the probability that an intensified version (storyline-projected) of it occurred in the future.

Applied to the 2018 Central European heatwave, storylines show an area-mean warming rate of 1.7 °C per degree of global warming. Through the flow-analogue method, it was evidenced that the atmospheric blocking leading to this event remains equally likely to occur regardless of global warming. Despite it, the storyline-projected intensities might become more frequent and extreme at their corresponding warming levels than the factual 2018 event was under present conditions. Specifically, the 2018 heatwave, with an intensity of 2.2 °C and a return period of 1-in-277-years today, is projected to intensify to 6.6 °C with a 1-in-26-years return period in a +4K world. This behavior revealed the importance of other physical mechanisms and interactions influencing the occurrence and intensification of heatwaves beyond the atmospheric circulation pattern and thermodynamic conditions. We conclude that this combined framework is promising for climate change attribution of individual extreme events, offering both a physical assessment of anthropogenic warming and its associated likelihood while accounting for potential shifts in atmospheric dynamics.

How to cite: León-FonFay, D., Lemburg, A., Fink, A. H., Pinto, J. G., and Feser, F.: A combined storyline-statistical approach for conditional attribution of climate extremes to global warming, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14325, https://doi.org/10.5194/egusphere-egu26-14325, 2026.

EGU26-14525 | Posters on site | CL3.2.4

Extreme weather events in agriculturally important regions in the Bay of Bengal 

Martina Messmer, Santos José González-Rojí, and Sonia Leonard

The Bay of Bengal is one of the most densely populated regions globally, bordered by India, Bangladesh, and Myanmar. Its coastal zones represent critical hotspots from both societal and agricultural perspectives. Major river deltas, including those of the Brahmaputra and Ganges in Bangladesh, the Mahanadi in India, and the Ayeyarwady in Myanmar, provide essential freshwater resources that sustain highly productive agricultural systems and support large local populations. However, ongoing climate change is increasingly associated with extreme weather conditions, such as elevated temperatures, prolonged droughts, and intense precipitation events.

To investigate how climate change at different time horizons and levels of warming influences these extremes, we conducted five regional climate simulations using the Weather Research and Forecasting (WRF) model at 5km horizontal spacing. One simulation represents a 30-year reference period (1981–2010). Two additional simulations cover the mid-21st century (2031–2060) under the SSP2-4.5 and SSP5-8.5 scenarios, respectively. The remaining two simulations represent the late 21st century (2071–2100) under the same SSP2-4.5 and SSP5-8.5 emission pathways.

The results indicate a substantial increase in extreme heat across all river deltas. The number of days exceeding 40 °C is projected to double under SSP2-4.5 and to triple under SSP5-8.5 by the end of the century. Drought frequency increases markedly, with the number of drought events projected to quadruple under both scenarios. Concurrently, extreme precipitation, measured by the RX5 index, shows significant increases in the Ayeyarwady and Brahmaputra deltas. The combined effects of intensified heat stress, more frequent droughts, and increasingly severe precipitation events present major challenges for both local populations and agricultural systems, potentially increasing the risk of displacement in these vulnerable regions.

How to cite: Messmer, M., González-Rojí, S. J., and Leonard, S.: Extreme weather events in agriculturally important regions in the Bay of Bengal, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14525, https://doi.org/10.5194/egusphere-egu26-14525, 2026.

EGU26-14618 | ECS | Orals | CL3.2.4

Evolution of global climate and regional hot extremes following CO2 emissions cessation. 

Andrea Rivosecchi, Andrea Dittus, Ed Hawkins, Reinhard Schiemann, and Erich Fischer

Reaching net zero greenhouse gas emissions is essential to halt the current global warming trend and attempt to stabilise global temperatures. However, uncertainties remain on the sign and the magnitude of the long-term responses of the climate system following anthropogenic emissions cessation.

This study contributes to constraining this uncertainty by exploring the global and regional temperature evolution under zero CO2 emissions conditions in the UKESM1.2 projections following the TIPMIP protocol (Jones et al., 2025). Stabilised warming levels spanning +1.5°C to +5°C above pre-industrial conditions are analysed to understand the impact of antecedent conditions on post zero-emissions trends. We find that the global average surface air temperature (GSAT) keeps increasing in all stabilised warming scenarios. The increase is more pronounced in the +3°C to +5°C scenarios, where it approaches 0.25°C per century. Most of the warming is registered in the Southern Hemisphere, particularly in the Southern Ocean, while the Northern Hemisphere experiences a slight cooling trend over land.

These regional cooling trends are more marked for the annual temperature maxima, with several regions across 45-65°N experiencing cooling of >1°C per century. The strongest cooling trends emerge in the higher warming scenarios, and we investigate their drivers in North America, where the cooling magnitude exceeds 1.5°C per century. Using a method based on constructed circulation analogues, we find that the projected cooling trend is almost completely explained by thermodynamic drivers and we reconcile this finding with the model vegetation changes. Our findings serve a double purpose. On one hand, they show the significant contribution that land-use changes can have regionally for the attenuation of annual temperature maxima, supporting the case for their careful consideration in future mitigation and adaptation strategies. On the other, they highlight how highly idealised protocols like TIPMIP could bias climate projections post emissions cessation if they do not include realistic projections of land use changes.

 

Bibliography

Jones, Colin, Bossert, I., Dennis, D. P., Jeffery, H., Jones, C. D., Koenigk, T., Loriani, S., Sanderson, B., Séférian, R., Wyser, K., Yang, S., Abe, M., Bathiany, S., Braconnot, P., Brovkin, V., Burger, F. A., Cadule, P., Castruccio, F. S., Danabasoglu, G., … Ziehn, T. (2025). The TIPMIP Earth system model experiment protocol: phase 1. https://doi.org/10.5194/egusphere-2025-3604.

How to cite: Rivosecchi, A., Dittus, A., Hawkins, E., Schiemann, R., and Fischer, E.: Evolution of global climate and regional hot extremes following CO2 emissions cessation., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14618, https://doi.org/10.5194/egusphere-egu26-14618, 2026.

In the aftermath of extreme weather, policy makers, contingency planners and insurers often seek to understand the likelihood of experiencing such events. The most common tool for this is extreme value analysis (EVA), but likelihood estimates based on observed or reanalysis data can be highly uncertain due to the relatively short observational record. Substantially larger samples of plausible extreme weather events can be obtained using the UNprecedented Simulated Extremes using ENsembles (UNSEEN) approach, which involves applying EVA to large forecast/hindcast ensembles. While larger sample sizes generally reduce the uncertainty associated with EVA, using seasonal or decadal forecast data introduces additional uncertainties related to model bias and model diversity. In this study, a multi-model ensemble of hindcast data from the CMIP6 Decadal Climate Prediction Project was analysed to quantify these additional uncertainties in the context of extreme temperature and rainfall across Australia. Factoring in model bias and diversity dramatically increased the uncertainty associated with estimated event likelihoods from the UNSEEN approach, to the point that it equaled or exceeded the uncertainty from an observation-based approach at most locations. Model diversity tended to be the largest source of uncertainty (60-70% of the total). Bias correction was also a significant source of uncertainty (30-40%), while the uncertainty associated with EVA was trivial. Our results suggest that an UNSEEN-based approach to estimating the likelihood of climate extremes should be understood as an approach that has different uncertainty characteristics to an observation-based approach, as opposed to less uncertainty.

How to cite: Irving, D., Stellema, A., and Risbey, J.: Quantifying the uncertainty associated with extreme weather likelihood estimates derived from large model ensembles, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14625, https://doi.org/10.5194/egusphere-egu26-14625, 2026.

EGU26-14884 | ECS | Posters on site | CL3.2.4

Emerging intra-annual sequences of climate extremes in Europe  

Andrea Böhnisch, Matthew Lee Newell, Ophélie Meuriot, Jorge Soto Martin, Ane Carina Reiter, and Martin Drews

Climate change drives an increase in the frequency of multiple meteorological extreme event types (e.g., extreme precipitation, storms, droughts, heatwaves) by affecting thermodynamic and dynamic processes in the coupled land-atmosphere system. For example, the extended droughts during 2018-2020 in Europe, flooding triggered by extreme precipitation in Germany in 2021, as well as Valencia and central France in 2024, or prolonged heatwaves in 2003, 2015, 2018, and 2022 across continental Europe had strong adverse impacts on socio-economic systems and the environment. Given a higher frequency of extreme events, it becomes more likely that regions experience events of the same or different types in consecutive seasons, thereby challenging the regions’ short-term coping and recovery ability and long-term resilience.

While extreme events are generally well-studied, holistic analyses of typical sequences of extreme events are missing. Compound analyses commonly focus on specific combinations of events, but usually miss typical intra-annual sequences of extreme events with the potential for high impacts.

Our analysis addresses the question 1) which sequences of extremes occur most often, 2) how robust they are, and 3) their physical implications. We assess intra-annual sequences of extreme seasons on the European scale in a regional multi-member ensemble of the Canadian Regional Climate Model version 5 (CRCM5) covering the European CORDEX domain at a high spatial resolution (0.11°, 12 km). The CRCM5 was driven by four members of the Max-Planck-Institute Grand Ensemble (MPI-ESM-LR) under SSP3-7.0. Given that the four members differ only by initial conditions and thus share the same climate, this setup quadruples the sample size for finding extreme events. We selected extreme event indicators for extreme heat, droughts, extreme precipitation and wind. They cover hazards of regionally varying importance, but each of them poses considerable risks to human and natural systems in Europe. The sequences of extreme events were derived using the sequential pattern mining algorithm cSPADE.

In this contribution, we show first findings on the most prevalent sequences of seasonal events under SSP3-7.0. We map vulnerability hotspots associated with intra-annual extreme event characteristics and present physical “stories” corresponding to the sequences. Furthermore, we aim to provide the basis for understanding potential interrelations of seasonal extreme events.

How to cite: Böhnisch, A., Lee Newell, M., Meuriot, O., Soto Martin, J., Reiter, A. C., and Drews, M.: Emerging intra-annual sequences of climate extremes in Europe , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14884, https://doi.org/10.5194/egusphere-egu26-14884, 2026.

EGU26-15041 | ECS | Orals | CL3.2.4

Amplified socioeconomic impacts of compound drought–heatwave events 

Koffi Worou and Gabriele Messori

Isolated and compound climate extremes, such as droughts and heatwaves, are intensifying under global warming. Although recent studies have advanced the physical understanding and classification of compound events, their socioeconomic impacts remain poorly quantified at the global scale using disaster record databases. Building on evidence that compound drought–flood events can generate impacts substantially larger than those from isolated hazards, this study extends the inquiry by providing a global assessment of the socioeconomic impacts of compound drought–heatwave (CDH) events.

To achieve this, we use the Emergency Events Database (EM-DAT) for the period 1960–2025 and analyse reported drought and heatwave disasters at the global scale. CDH events are identified using complementary approaches, including overlapping drought and heatwave records within the same location (top-level administrative unit) and the “Associated Types” information in EM-DAT, thereby allowing assessment of sensitivity to event definition. Furthermore, EM-DAT drought events are compared with heatwave conditions derived from the ERA5 reanalysis to evaluate consistency between reported impacts and climatic co-occurrence. Socioeconomic impacts are quantified using the affected population, human fatalities, and reported damages.

Preliminary results show a clear increase in the number of reported areas affected by CDH events globally, particularly since the mid-2010s. Moreover, CDH events are consistently associated with greater impacts than single hazards. Specifically, using matching events within EM-DAT, compound events exhibit greater total damage, while fatalities during heatwaves increase by up to a factor of five when drought conditions co-occur. Furthermore, when drought impacts from EM-DAT are associated with heatwaves identified in ERA5, the damage and affected population are, respectively, two to four times higher than for isolated drought events.

Taken together, these findings provide global-scale evidence that co-occurring droughts and heatwaves substantially amplify socioeconomic impacts. This underscores the need to explicitly account for compound extremes in climate risk assessment, adaptation planning, and disaster risk reduction.

How to cite: Worou, K. and Messori, G.: Amplified socioeconomic impacts of compound drought–heatwave events, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15041, https://doi.org/10.5194/egusphere-egu26-15041, 2026.

EGU26-15607 | ECS | Orals | CL3.2.4

Intensification of Short-Duration Extreme Precipitation in Greater Sydney 

Leena Khadke, Jason P. Evans, Youngil Kim, Giovanni Di Virgilio, and Jatin Kala

Short-duration extreme precipitation is a key driver of urban flooding and associated socio-economic impacts in a warming climate. Increasing urbanization further amplifies the vulnerability of cities to intense rainfall occurring over minutes to hours. These extremes frequently trigger flash floods and pose substantial risks to urban infrastructure and public safety. Despite growing recognition of its importance, regional-scale assessments of sub-hourly extreme precipitation remain limited. Emerging observational evidence indicates that short-duration precipitation events (≤1 hour) are intensifying at a faster rate than longer-duration events. In this study, we analyze short-duration extreme precipitation events at 5-, 10-, 20-, 30-, and 60-minute timescales using observations from 16 automated weather stations (AWS) across the rapidly urbanizing Greater Sydney region, New South Wales, Australia. Our results show a pronounced increasing trend in extreme precipitation at higher percentiles, particularly at the 5–10 minute timescales, compared to hourly extremes. At the hourly scale, we evaluate the performance of five convection-permitting regional climate model simulations (4 km ensemble) against AWS observations. The models reasonably capture the upper tail of the precipitation distribution but tend to slightly overestimate the frequency of extreme events. To assess future changes, we examine the intensity of 99th percentile precipitation extremes across three periods—historical (1951–2014), near future (2015–2057), and far future (2058–2100)—under three Shared Socioeconomic Pathway scenarios (SSP126, SSP245, and SSP370). The projections indicate a consistent intensification of extreme precipitation, with a substantial upward shift in the top 1% of historical extremes, most pronounced under the high-emission SSP370 scenario. Interestingly, the simulations also project a reduction in the total number of wet hours relative to the historical baseline, suggesting a transition toward shorter-duration but more intense precipitation events. Although considerable inter-model spread and spatial variability exist, increases in 99th percentile extremes are robust across most scenarios. Notably, under SSP126, a decline in extreme precipitation is projected in the far future, highlighting the potential benefits of strong emission mitigation. These findings underscore the need to explicitly incorporate short-duration precipitation extremes into urban planning and flood risk management under climate change.

Keywords: Automatic Weather Station, Climate change, Flash floods, NARCliM2.0, Regional climate models, Sub-hourly extreme precipitation

How to cite: Khadke, L., Evans, J. P., Kim, Y., Virgilio, G. D., and Kala, J.: Intensification of Short-Duration Extreme Precipitation in Greater Sydney, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15607, https://doi.org/10.5194/egusphere-egu26-15607, 2026.

On 1 October 2020, the intense extra-tropical storm Alex impacted the north-west coast of France, producing unusually strong wind gusts for the season. On 2 October, the storm triggered record-breaking rainfall over the south-eastern French Alps and north-western Italian Alps. In France, this Heavy Precipitation Event (HPE) caused severe flooding and land­slides, resulting in casualties, and over 1 billion euros in economic losses.

We used convection-permitting regional climate modeling with a spa­tial resolution of 2.5 km to investigate these observed events. Simulations were conducted over September-October 2020 on an extensive domain centered on France. Our model successfully reproduces the characteristics of both the HPE and storm Alex, including the observed sequence of events and impacts (Bador et al., 2025).

We then explored how the observed 2020 Mediterranean HPE could have been differ­ent had it occurred 2 years later, in 2022, where warmer sea surface was recorded in the western Mediterranean Sea. This storyline analysis suggested reduced precipitation impacts over the south-eastern French Alps but enhanced impacts in Italy. Additional sensitivity experiments confirmed the key role of regional sea surface temperatures (SSTs) in shaping the HPE’s intensity in the western Alps, with an eastward shift of heavy precipitation with higher Mediterranean SSTs. Our simulations consistently show that sea surface warming can further intensify the Mediterranean HPE, while cooling reduces the intensity of extreme precipitation and local impacts. In contrast, modifications to the Atlantic SSTs affecting storm Alex itself have a limited influence on the regional Mediterranean circulation and the HPE.

All simulations were performed using initial-condition large ensembles to assess the role of internal variability in shaping local extremes. We highlighted variations among ensemble members in both local rainfall extremes and in gustiness. As impact sectors increasingly rely on km-scale climate modelling to inform local climate change assessments, our results underscore the importance of the ensemble-based approaches to fully capture the range of possible outcomes for extreme events locally.

How to cite: Bador, M., Noirot, L., Caillaud, C., and Boé, J.: Cooler than observed sea surface could have reduced impacts of storm Alex and induced mediterranean heavy precipitation event in France, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16649, https://doi.org/10.5194/egusphere-egu26-16649, 2026.

EGU26-16825 | Orals | CL3.2.4

 Trends and Drivers of Cold Extremes in a Changing Climate 

Daniela Domeisen, Hilla Afargan-Gerstman, Russell Blackport, Amy H. Butler, Edward Hanna, Alexey Yu. Karpechko, Marlene Kretschmer, Robert W. Lee, Amanda Maycock, Emmanuele Russo, Xiaocen Shen, and Isla R. Simpson

Cold extremes — also referred to as cold air outbreaks, cold spells, or cold snaps — have received less attention in the scientific literature than hot extremes, largely because their frequency and intensity are projected to decrease under climate change. Nevertheless, cold extremes continue to exert substantial impacts across a wide range of sectors, including human health, agriculture, and infrastructure. Superimposed on their overall global decline is pronounced regional and seasonal variability, driven by variability in the underlying physical mechanisms, which themselves may be influenced by climate change. Here, we provide an overview of global and regional trends in cold extremes, examine their key drivers in both present and future climates, and discuss outstanding questions related to the dynamical forcing of cold extremes and their projected evolution under climate change.

How to cite: Domeisen, D., Afargan-Gerstman, H., Blackport, R., Butler, A. H., Hanna, E., Karpechko, A. Yu., Kretschmer, M., Lee, R. W., Maycock, A., Russo, E., Shen, X., and Simpson, I. R.:  Trends and Drivers of Cold Extremes in a Changing Climate, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16825, https://doi.org/10.5194/egusphere-egu26-16825, 2026.

The increasing frequency of extreme hot events poses major societal and scientific challenges due to their adverse impacts on human and natural systems, compounded by their unpredictable nature. Climate models are essential for identifying the mechanisms that amplify extremes and for anticipating long-term changes that inform decision making, yet their accuracy is limited by internal variability, structural uncertainties, and systematic biases. Observational constraint approaches that link past and future behavior of physical observables offer a promising way to address these limitations, though they often rely on region-specific empirical relationships.

Here, we show that future changes in hot event probabilities and their uneven spread across global land areas depend critically on the historical properties of temperature distributions. In particular, historical variability controls the growth rates of probabilities, either amplifying or dampening the effects of regional background warming, with important implications for climate-change projections. Building on this insight, we develop a universal analytical framework that combines observational evidence with model output to provide more robust assessments of future changes. Results indicate that hot event probabilities may increase faster than suggested by models alone across much of the land surface. In large areas, including the Euro-Mediterranean and Southeast Asia, observation-constrained increases could exceed model-based estimates by nearly a factor of two, even at low levels of global warming. Surpassing the 2 °C warming threshold could push highly vulnerable regions, such as the Amazon and other tropical land areas, into uncharted climate conditions where extreme heat becomes routine.

These findings support more realistic evaluations of future risk and underscore the need for strengthened mitigation efforts to prevent rapid and potentially irreversible climate shifts.

How to cite: Simolo, C. and Corti, S.: Hot extremes increase faster than models suggest: evidence from observation-constrained projections, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17562, https://doi.org/10.5194/egusphere-egu26-17562, 2026.

EGU26-18203 | ECS | Orals | CL3.2.4

Heat extremes in subseasonal hindcasts: a General Extreme Value perspective 

Pauline Rivoire, Maria Pyrina, Philippe Naveau, and Daniela Domeisen

Understanding and characterizing temperature extremes is essential for assessing climate impacts and risks. Robust statistical analysis of such extremes requires large datasets, yet observational records often provide limited samples of rare events. Hindcasts, i.e., retrospective forecast model runs for past dates, are typically used to correct model biases, but their potential for extreme event analysis remains underexplored. Approaches such as UNSEEN (UNprecedented Simulated Extremes using Ensembles) have investigated the potential of seasonal hindcast ensembles to provide large samples of events that are physically plausible, particularly for assessing rare events. However, seasonal hindcasts often focus on monthly means.

In this study, we explore whether a similar approach can be applied to subseasonal hindcasts, evaluating their potential to serve as alternative realizations of extreme events at daily resolution.  We use two complementary methods to compare global temperature extremes in ECMWF subseasonal hindcast with ERA-5 reanalysis: (1) the statistical upper bound of daily 2-meter temperature, and (2) the probability of record-breaking daily 2-meter temperature. By leveraging existing subseasonal hindcast ensembles, we aim to evaluate whether these datasets can be repurposed to study temperature extremes that have not yet been observed but are plausible under current climate conditions

How to cite: Rivoire, P., Pyrina, M., Naveau, P., and Domeisen, D.: Heat extremes in subseasonal hindcasts: a General Extreme Value perspective, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18203, https://doi.org/10.5194/egusphere-egu26-18203, 2026.

Unclear and inconsistent terminology for high impact climate phenomena, including concepts such as tipping points, irreversibility, ‘collapse’ and ‘shutdown’, presents a substantial barrier to clear understanding of Earth system risks. These terms are frequently used in assessments of major subsystem shifts in ocean circulation, ice sheets and forest biomes, yet they are often applied without shared definitions across scientific, policy and public contexts. This inconsistency affects how scientific results are interpreted, including perceptions of how quickly changes may unfold and whether different parts of the climate system might influence one another. It also has important psychological and emotional impacts. Language that sounds dramatic or alarming may be intended to motivate action, but it can instead lead to desensitisation, message fatigue, denial or even the spread of misinformation. These reactions can weaken engagement and undermine societal preparedness for potential climate driven transitions.

Government science and policy teams, rely on clear and consistent terminology for effective decision making in situations where thresholds and impacts remain uncertain. To support this need, we – as communication specialists work extensively at the interface between science and policy - are developing an evidence-based glossary and guidance for terminology related to tipping points and other high impact climate concepts. The aim is to improve internal communication and to support clearer interpretation of scientific assessments used in national risk planning.

The project is grounded in social science and uses a mixed methods design. It began with a review of existing definitions and research on the psychological effects of climate language. We carried out semi-structured interviews and workshops with scientists and government officials, and this highlighted how linguistic ambiguity affects policy development and the evaluation of uncertain risks. Utilising ta broad cross section of Met Office staff, we carried out focus groups to explore how different definitions were perceived and understood. Participants, including those with strong scientific backgrounds, showed substantial disagreement about the meaning and implications of key terms. This indicates that confusion around terminology linked to tipping point research is not limited to public audiences but also exists within expert communities.

Insights from this analysis are guiding the co creation of a public facing glossary developed with an expert working group of twelve multidisciplinary specialists at the Met Office. Completion is planned for March 2026, alongside continued engagement with international bodies including WCRP and IPCC. By strengthening shared understanding of terms related to climate system transitions and critical thresholds, this work aims to support more coherent communication of high impact climate concepts, improve public and policy interpretation of uncertain risks and reduce unintended emotional and behavioural responses that can undermine, and distract from effective, and much needed climate action.

How to cite: Macneill, K. and Martin, L.: An Up-HILL Battle: Building consensus on terminology for high impact climate events and tipping point risks., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18736, https://doi.org/10.5194/egusphere-egu26-18736, 2026.

EGU26-19875 | ECS | Posters on site | CL3.2.4

Using Stochastic Data to Simulate and Communicate Alternative Multi-Hazard Weather Extreme Events 

Judith Claassen, Wiebke Jäger, Marleen de Ruiter, Elco Koks, and Philip Ward

A stochastic weather generator (SWG) simulates realistic weather time series beyond the historical record by capturing the statistical properties of observed weather patterns. Here, we present a new spatiotemporal SWG, the MYRIAD Stochastic vIne-copula Model (MYRIAD-SIM), which simulates temperature, wind speed, and precipitation. MYRIAD-SIM captures both spatiotemporal and multivariate dependencies using conditional vine copulas. The simulated data enable new insights into compound climate and multi-hazard events by generating high-impact multivariate weather scenarios. For example, the triple storm sequence Dudley, Eunice, and Franklin, which impacted the UK and Europe in 2022, can be simulated as alternative triple-storm events, illustrating not only what happened but also what could have occurred under statistically plausible conditions, such as higher wind speeds or varying precipitation patterns. This study demonstrates how stochastic counterfactuals of historical events can support risk communication by framing hazards in a narrative, event-focused way rather than through abstract probabilities.

How to cite: Claassen, J., Jäger, W., de Ruiter, M., Koks, E., and Ward, P.: Using Stochastic Data to Simulate and Communicate Alternative Multi-Hazard Weather Extreme Events, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19875, https://doi.org/10.5194/egusphere-egu26-19875, 2026.

EGU26-19952 | ECS | Posters on site | CL3.2.4

Circulation pathways and surface drivers of extreme summer heat stress over Europe 

Qi Zhang, Joakim Kjellsson, and Emily Black

Extreme summer heat stress presents increasing public health risks across Europe. These extremes are strongly influenced by large-scale atmospheric circulation, yet the specific pathways linking circulation evolution to surface heat stress amplification remain poorly understood. Using the simplified Wet Bulb Globe Temperature (sWBGT), which accounts for both temperature and humidity effects on heat stress, we analyze extreme summer (JJA) events during 1979–2023 based on ERA5 reanalysis and a seven-class European weather regime (WR) classification. We define extreme events as regional sWBGT exceeding the 95th percentile for at least three consecutive days. Extreme sWBGT events across Europe occur predominantly during blocking regimes, with European and Scandinavian blocking playing a dominant role in many regions. We then examine how blocking evolves prior to heat stress peaks. Results show that only Scandinavia exhibits a statistically robust tendency for blocking to develop shortly before the peak, suggesting a circulation transition preceding extreme heat stress. In contrast, most other European regions experience peak heat stress under blocking conditions that are already established several days in advance, highlighting the dominant role of persistent circulation patterns. The time interval between the onset of blocking and the heat stress peak typically ranges from 3 to 7 days. These contrasting circulation pathways are closely linked to different surface amplification processes. Circulation transitions maybe associated with rapid atmospheric adjustment and surface warming, whereas persistent blocking likely promotes the accumulation of radiative forcing and progressive soil moisture depletion. Understanding how these mechanisms vary across pathways can help explain regional differences in European heat stress extremes and may improve predictions of future events.

How to cite: Zhang, Q., Kjellsson, J., and Black, E.: Circulation pathways and surface drivers of extreme summer heat stress over Europe, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19952, https://doi.org/10.5194/egusphere-egu26-19952, 2026.

EGU26-20226 | Orals | CL3.2.4

Robust and actionable information on climate change and extreme rainfall events in South America 

Alice M Grimm, Lucas G Fanderuff, and João P J Saboia

Obtaining robust and actionable information on regional precipitation change to enable adaptation planning and decision-making is a matter of great concern, since there are multiple sources of information.  Projections from large CMIP6 model ensembles (e.g., IPCC Interactive Atlas) show weak signal of climate change in total annual and seasonal precipitation over most of South America (SA), with low agreement between models. Besides, information from smaller ensembles is frequently discrepant. A dynamic framework for climate change in SA is necessary to achieve robust and actionable changes.

Even though they are weak and not robust, the precipitation changes produced over SA by large model ensembles suggest that their main driver is the ENSO increased variability in eastern Pacific, especially intensified El Niño events, produced by transient greenhouse-gas-induced warming. This is consistent with the large impact of ENSO on precipitation in SA. This dynamical framework requires that models used for climate projections in SA demonstrate good simulation not only of the climatology, but also of ENSO and its teleconnections with SA. The assessment of 31 models that provided at least three runs from the present (1979-2014) to the future climate (2065-2100), based on both criteria, selected five best-performing models. This reduced set accurately reproduces the observed seasonal impact of ENSO on precipitation in SA and produces strong and robust patterns of climate change with seasonal variation dynamically consistent with more intense future ENSO in a more El Niño-like mean state.

Since the most dramatic impacts of climate change are produced by changes in the frequency and intensity of extreme precipitation events, it is essential that robust and actionable information is also provided on changes of these events, defined as above the 90th percentile. The analysis is based on the same dynamic framework of the changes in total seasonal/monthly rainfall, since ENSO also exerts a large impact on the extreme events in SA, and the selected set of models shows good simulation of the observed seasonal/monthly impact of ENSO on the frequency and intensity of extreme events. The available information usually shows changes of annual extreme indices. We adopt a seasonal/monthly resolution, which is very useful, especially in a monsoon regime with pronounced annual precipitation cycle. The future changes in extreme events is obtained for SA with monthly temporal resolution and 1 degree spatial resolution. The patterns of change in frequency and intensity of extreme events do not coincide, as changes in frequency depend on dynamic changes, while changes in intensity also depend on thermodynamic changes that determine the precipitable water vapor. Patterns of change in the frequency of extreme events in future are similar to the patterns of El Niño impact on the frequency of extreme events in the present. Changes in the average intensity of precipitation in future extreme events are generally positive and predominate in southeastern South America, where the frequency also generally increases, maximizing impacts on densely populated areas of great importance for agricultural and energy production. The provided information contributes to increase societal preparedness to extreme precipitation in SA.

How to cite: Grimm, A. M., Fanderuff, L. G., and Saboia, J. P. J.: Robust and actionable information on climate change and extreme rainfall events in South America, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20226, https://doi.org/10.5194/egusphere-egu26-20226, 2026.

EGU26-21160 | ECS | Posters on site | CL3.2.4

The influence of soil moisture on the extreme precipitation event in July 2021 in Western Europe 

Till Fohrmann, Svenja Szemkus, Oliver Heuser, Arianna Valmassoi, and Petra Friederichs

Soil moisture-precipitation feedback is an important factor in the water and energy cycles, but how important is it on the time scale of an atmospheric extreme precipitation event? We are investigating this question using the example of heavy precipitation in July 2021, which led to destructive flash floods in Western Europe.

We quantify the importance of soil moisture by running a storyline simulation. We compare the precipitation simulated in the ICON-DREAM reanalysis and in our control run to counterfactual scenarios with soils dried out to plant wilting point and soils wetted to saturation. We find that saturating the soil increases precipitation by about 10% while drying the soil decreases precipitation by about 36% comparing ensemble median values.

Moisture tracking shows that one reason is that land surfaces in the vicinity of the impacted region are relevant for fueling the heavy precipitation. We find that evaporation is not limited by water availability, which explains the non-linear response in the precipitation amounts. 

The changes in evaporation also affect the synoptic scale evolution of the event, which amplify the precipitation decrease in the dry scenario. Constraining the evolution of the event enough to produce the extreme of July 2021 was a major challenge of this study. The limited predictability of free forecasts conflicts with the need for enough lead time to allow soil moisture to impact the atmosphere in a meaningful way. We solve this problem by using data assimilation to constrain the large scale circulation of our global ICON simulations while disabling the assimilation within our region of interest.

Our work is part of the German Research Foundation (DFG) Collaborative Research Center 1502 DETECT. In DETECT we aim to answer the question of whether regional changes in land and water use impact the onset and evolution of extreme events. Our coarse approach to changes in water availability gives us an upper bound on changes we can expect as a result of human influence.

How to cite: Fohrmann, T., Szemkus, S., Heuser, O., Valmassoi, A., and Friederichs, P.: The influence of soil moisture on the extreme precipitation event in July 2021 in Western Europe, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21160, https://doi.org/10.5194/egusphere-egu26-21160, 2026.

EGU26-21435 | ECS | Orals | CL3.2.4

Robust response of Antarctic sea ice to large-scale wind anomalies across different climate backgrounds 

Lingyun Lyu, Antonio Sánchez-Benítez, Marylou Athanase, Lettie A. Roach, Thomas Jung, and Helge F. Goessling

Antarctic sea ice has experienced small increases from 1979 to 2015, followed by an unexpectedly rapid decline reaching record-low anomalies in 2016 and 2023. The significant reduction is raising questions regarding the drivers of this decline and how the Antarctic sea ice will respond to future climate changes. Here we apply an event-based storyline approach based on a coupled global climate model (AWI-CM-1-1-MR), where the large-scale free-troposphere dynamics is constrained to ERA5 data. We focus on two multi-year sea-ice loss events, 2014–2017 and 2020–2023, to examine the response of sea ice to the observed atmospheric circulation anomalies if they occurred under different global climate backgrounds. By comparing the sea-ice response under present-day climate and projected future warm climates (+2°C, +3°C, and +4°C global mean surface warming relative to preindustrial), we separate the thermodynamic and dynamic effects of climate change and explore how the background climate state modulates the sea-ice response to wind anomalies. We find that the Antarctic sea-ice response remains surprisingly robust across this broad range of climate states, with a few exceptions where seasonal and regional deviations occur.

How to cite: Lyu, L., Sánchez-Benítez, A., Athanase, M., A. Roach, L., Jung, T., and F. Goessling, H.: Robust response of Antarctic sea ice to large-scale wind anomalies across different climate backgrounds, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21435, https://doi.org/10.5194/egusphere-egu26-21435, 2026.

NP2 – Dynamical Systems Approaches to Problems in the Geosciences

EGU26-673 | PICO | NP2.1

Critical Transitions at Campi Flegrei Resurgent Caldera: A Novel Approach to Systemic and Retrospective Signals Analysis 

Andrea Vitale, Andrea Barone, Enrica Marotta, Dino Franco Vitale, Susi Pepe, Rosario Peluso, Raffaele Castaldo, Rosario Avino, Francesco Mercogliano, Antonio Pepe, Filippo Accomando, Gala Avvisati, Pasquale Belviso, Eliana Bellucci Sessa, Carandente Antonio, Perrini Maddalena, Fabio Sansivero, and Pietro Tizzani

This study investigates how complex volcanic systems undergo major behavioral shifts, focusing on the Solfatara–Pisciarelli (SP) hydrothermal-magmatic area within the Campi Flegrei caldera (Southern Italy). The SP system is one of the most active zones of the caldera, characterized by persistent degassing, seismic swarms, strong hydrothermal circulation and long-term ground uplift. These processes arise from nonlinear interactions between magmatic inputs, fluid migration, and shallow hydrothermal pressurization, making the identification of critical transitions particularly challenging.

To address this, we developed an integrated analytical framework combining Multivariable Fractional Polynomial Analysis (MFPA) and Global Critical Point Analysis (GCPA). MFPA models nonlinear and time-lagged associations among key monitoring parameters—vertical ground deformation, seismicity, CO₂ flux, geochemical equilibrium variables, and thermal signals—while GCPA identifies the temporal moments when multiple variables collectively show systemic reorganization.

Analysis of multi-year (2018–2024) geophysical and geochemical datasets revealed that deformation is strongly associated with seismicity, equilibrium pressures of hydrothermal gases, heat flow, and CO₂ flux. Incorporating time-lagged deformation improved model accuracy and reduced unexplained variance, highlighting delayed cause–effect couplings between deformation and fluid-dynamic processes. The model confirms seismicity as the most stable explanatory parameter, consistent with sustained fracturing and fluid pressurization in the shallow system.

GCPA identified two major critical transitions:

  • CP1 – 30 November 2020, dominated by thermal–chemical reorganization and increased gas-system pressurization.
  • CP2 – 1 April 2023, reflecting a more open and multiparametric regime where deformation, temperature, seismicity, heat flux, and CO₂ emissions contribute comparably to system evolution.

These transitions align with independent geodetic evidence suggesting migration and reconfiguration of the shallow overpressure source beneath the SP area. The integrated MFPA–GCPA approach thus reconstructs how systemic changes propagate across geophysical and geochemical variables, providing retrospective insight into the onset and progression of unrest phases.

This framework offers several advantages over classical or non-parametric approaches: interpretability of functional relationships, explicit treatment of nonlinearities and time lags, and the ability to detect collective regime shifts rather than isolated anomalies. Although not predictive, the method provides a quantitative basis for identifying critical phases in volcanic systems and may be adapted to other densely monitored calderas. With higher-resolution and real-time data streams, it could support early indications of evolving unrest and enrich next-generation volcano-monitoring strategies.

How to cite: Vitale, A., Barone, A., Marotta, E., Vitale, D. F., Pepe, S., Peluso, R., Castaldo, R., Avino, R., Mercogliano, F., Pepe, A., Accomando, F., Avvisati, G., Belviso, P., Bellucci Sessa, E., Antonio, C., Maddalena, P., Sansivero, F., and Tizzani, P.: Critical Transitions at Campi Flegrei Resurgent Caldera: A Novel Approach to Systemic and Retrospective Signals Analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-673, https://doi.org/10.5194/egusphere-egu26-673, 2026.

EGU26-2991 | ECS | PICO | NP2.1

How different are parameterisation packages really and how can we interpret stochastic perturbations? 

Edward Groot, Hannah Christensen, Xia Sun, Kathryn Newman, Wahiba Lfarh, Romain Roehrig, Lisa Bengtsson, and Julia Simonson

In the Model Uncertainty-Model Intercomparison Project (MUMIP) we compare parameterisation packages from different modelling centres using their single-column modelling (SCM) frameworks. We will showcase the dataset from an Indian Ocean experiment at a 0.2 degrees grid covering one month, with about 10 million simulations of each model. These parametrised models are compared against a convection-permitting benchmark from DYAMOND under common dynamical constraints. We will show differences and similarities in precipitation patterns and physics tendencies among four models and show how these differences can be generalised. Following earlier works, we find that at coarse grids that do not resolve convection, parameterisation packages tend to produce overconfident tendencies compared to the convection-permitting benchmark. Furthermore, we test several hypotheses on the MUMIP dataset to explain the differences. We use the data to explore the foundations of stochastic physical parametrisations. Would stochastic physics effectively overcome the overconfidence for good reasons? May the stochastic perturbations actually have a physically meaningful quantitative interpretation? Can stochastic physics be used to partially overcome truncation and grid spacing limitations?

How to cite: Groot, E., Christensen, H., Sun, X., Newman, K., Lfarh, W., Roehrig, R., Bengtsson, L., and Simonson, J.: How different are parameterisation packages really and how can we interpret stochastic perturbations?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2991, https://doi.org/10.5194/egusphere-egu26-2991, 2026.

EGU26-3111 | ECS | PICO | NP2.1

New insights into decadal climate variability in the North Atlantic revealed by data-driven dynamical models 

Andrew Nicoll, Hannah Christensen, Chris Huntingford, and Doug Smith

The Atlantic Multidecadal Variability (AMV) and the North Atlantic Oscillation (NAO) are the dominant modes of oceanic and atmospheric variability in the North Atlantic, respectively, and are key sources of predictability from seasonal to decadal timescales. However, the physical processes and feedback mechanisms linking the AMV and NAO, and the role of diabatic processes in these feedbacks, remain debated. We present a data-driven dynamical modelling framework which captures coupled decadal variability in AMV, NAO, and North Atlantic precipitation. Applying equation discovery methods to observational data, we identify deterministic low-order dynamical models consisting of three coupled ordinary differential equations. These models reproduce observed North Atlantic decadal variability and show robust out-of-sample predictive skill on multi-annual to decadal lead times. The resulting model dynamics include a distinct quasi-periodic 20-year oscillation consistent with a damped oceanic mode of variability. Notably, precipitation-related terms feature prominently in the low-order models, suggesting an important role for latent heat release and freshwater fluxes in mediating ocean–atmosphere interactions. We propose new feedback mechanisms between North Atlantic sea surface temperature and the NAO, with precipitation acting as a dynamical bridge. By linearising the low-order models and computing finite-time Lyapunov exponents, we find that North Atlantic precipitation is more predictable in a positive AMV phase. We then analyse several decadal prediction ensemble experiments based on initialised hindcasts and find comparable state-dependent predictability of precipitation. Overall, these results illustrate how data-driven equation discovery can provide mechanistic hypotheses and new insight beyond conventional analyses of observations and climate model simulations.

How to cite: Nicoll, A., Christensen, H., Huntingford, C., and Smith, D.: New insights into decadal climate variability in the North Atlantic revealed by data-driven dynamical models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3111, https://doi.org/10.5194/egusphere-egu26-3111, 2026.

Ensemble forecast generate multiple predictions from a set of initial conditions, thereby producing the probability density distribution (PDF) of a variable and quantifying forecast uncertainty beyond a single deterministic forecast. However, studies focusing on the predictable lead time of ensemble forecast remain limited. In this study, orthogonal conditional nonlinear optimal perturbations (O-CNOPs) are applied to the Lorenz-96 model to investigate the predictable lead time of ensemble forecast, which is then compared with that obtained from a single deterministic forecast. Results show that the maximum predictable lead time revealed by the ensemble distribution generated with O-CNOPs is 18.5 days, 2.5 days longer than that revealed by the ensemble distribution generated with singular vectors (SVs), which is 16 days. Consistent results are obtained from the ensemble mean analysis, which reveals a longer predictable lead time for O-CNOPs (21.75 days) than for SVs (18 days). In addition, compared with ensemble forecasts generated with SVs, the ensemble forecasts generated with O-CNOPs exhibit higher deterministic forecast skill, probabilistic forecast skill, reliability, and resolution over the same forecast periods. These results collectively highlight the advantage of O-CNOPs in constructing physically consistent nonlinear ensemble distributions and provide a methodological framework for more accurate quantification of ensemble forecast lead time.

How to cite: Zhu, Y. and Duan, W.: Exploring the Predictable Lead Time of Ensemble Forecast Based on Conditional Nonlinear Optimal Perturbation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3320, https://doi.org/10.5194/egusphere-egu26-3320, 2026.

The skill of forecasting Tropical Cyclone (TC) Rapid Intensification (RI) is limited by inherent uncertainties in initial conditions and model physics. To address this, the C-NFSVs method integrates initial and model perturbations, accounting for their collective effects through the nonlinear forcing singular vector (NFSV; also known as CNOP-F) approach. In this study, we applied C-NFSVs to the Weather Research and Forecasting (WRF) model for TC ensemble forecasting across three resolutions, comparing it against O-NFSVs, which has proven superior to traditional stochastic physics schemes. Results reveal a significant resolution dependence, with the superiority of C-NFSVs maximizing at the convection-permitting scale. At this resolution, the C-NFSVs ensemble outperforms O-NFSVs for both deterministic and probabilistic metrics, and demonstrates significantly improved reliability. Notably, for the challenging prediction of RI events, C-NFSVs exhibits high discriminative skill, achieving an Area Under the ROC Curve (ROCA) of 0.80. A detailed examination of TC Hato attributes this success to capturing the evolution of the critical physical error chain, which progresses from thermodynamic priming and convective organization to the structural and dynamic response. Mechanistically, the results highlight the complementary roles of the two components: the initial component of C-NFSVs dominates the uncertainty of the dynamic structure in the early forecast stage, while the model component plays a primary role in maintaining the thermodynamic uncertainty of moisture and temperature fields throughout the forecast. This study validates the effectiveness and physical rationality of C-NFSVs in high-resolution ensembles, offering a promising strategy for enhancing the predictability of extreme weather events at convection-permitting scales.

 

How to cite: You, C. and Duan, W.: Enhancing Tropical Cyclone Ensemble Forecast Skill via the Collective Effect of Initial and Model Perturbations: The C-NFSVs Method, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3326, https://doi.org/10.5194/egusphere-egu26-3326, 2026.

EGU26-4547 | ECS | PICO | NP2.1

Reconstruction of Global Forest Aboveground Carbon Dynamics with Probabilistic Deep Learning 

Zhen Qian, Sebastian Bathiany, Teng Liu, Lana Blaschke, Hoong Chen Teo, and Niklas Boers

Understanding the long-term dynamics of forest aboveground carbon (AGC) is critical for constraining the terrestrial carbon cycle. However, accurately reconstructing historical AGC spatiotemporal patterns remains a challenge due to the complex, nonlinear relationships between vegetation proxies and biomass, as well as the stochastic uncertainties inherent in multi-source satellite observations.

In this study, we propose a probabilistic deep learning framework to reconstruct harmonized, high-resolution (0.25°) global forest AGC stocks and fluxes from 1988 to 2021. By integrating multi-source optical (e.g., NDVI, LAI) and microwave (e.g., VOD) remote sensing data, our approach utilizes Probabilistic Convolutional Neural Networks (CNNs) to simultaneously estimate AGC dynamics and quantify associated predictive uncertainties (decomposing aleatoric and epistemic components). This data-driven model effectively captures the nonlinear spatial dependencies and texture features that traditional empirical methods often miss.

Our reconstruction reveals significant decadal-scale regime shifts in the global forest carbon sink. While global forests remained a net sink of 6.2 PgC over the past three decades, we identify a pronounced transition in moist tropical and boreal forests, which have shifted from carbon sinks to sources since the early 2000s. Furthermore, our analysis uncovers an intensifying negative coupling between interannual tropical AGC fluxes and atmospheric CO2 growth rates (r=-0.63 in the last decade), suggesting a growing complexity in the climate-carbon feedback. Spatially explicit partitioning in the Amazon further indicates a dynamical shift where AGC losses are increasingly driven by indirect climate stressors in previously "untouched" forests, rather than direct deforestation alone.

In conclusion, this study elucidates the state-dependent responses of global forests to changing disturbance regimes. The probabilistic framework provides a necessary basis for distinguishing genuine regime shifts, such as the structural decline of the tropical carbon sink, from observation noise, thereby enhancing our predictive understanding of terrestrial carbon resilience in a warming climate.

How to cite: Qian, Z., Bathiany, S., Liu, T., Blaschke, L., Teo, H. C., and Boers, N.: Reconstruction of Global Forest Aboveground Carbon Dynamics with Probabilistic Deep Learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4547, https://doi.org/10.5194/egusphere-egu26-4547, 2026.

EGU26-5335 | PICO | NP2.1

Low-dimensional stochastic amplitude equations for a precessing rotating cylinder 

Uwe Harlander and Carsten Hartmann

The magnetic field of planets and stars is generated by the movement of conductive fluids inside these bodies. The precession and libration of these astrophysical bodies play a central role in the excitation of the internal turbulent fluid motion. In our laboratory, we have developed an experiment that allows the investigation of precession-driven inertial waves and their instability (Xu and Harlander, 2020). Wave triads play a very important role in this instability (Lagrange et al., 2011). As the Ekman number decreases, an increasing number of interacting triads arise, ultimately leading to turbulence. This process can be experimentally reproduced in the laboratory. In this experiment, precession is simulated using a slightly tilted cavity with a free fluid surface and is therefore simpler in design than a real precession experiment. 

The dynamics of fluids can be described by PDEs. However, often deeper insights can be gained from a corresponding low-dimensional dynamical system. An example is the large family of Lorenz-type models, which have led to a fundamental understanding of predictability in atmospheric dynamics (Majda et al., 1999). Also, for the problem of a precessing rotating cylinder, low-dimensional models exist. Such models are obtained from spectral discretizations of the Navier-Stokes equations and truncating the resulting hierarchy of coupled equations at low order. Truncation, however, eliminates the quadratic coupling between the resolved modes and the (unresolved) smaller scales, which can lead to unrealistic characteristics of turbulence. 

We suggest another closure to systematically derive low-order amplitude equations for rotating fluids, based on stochastic modeling of the unresolved small scales in accordance with the available experimental data. Specifically, we first remodel the small scales by an appropriate stochastic process that has a multivariate Gaussian law when conditioned on the resolved variables and, in a second step, apply a projection operator to the coupled system. In doing so, we derive closed, averaged equations for the resolved variables that retain the quadratic nonlinearities and so capture the small-scale contributions to the low-order wave dynamics. For a projection operator in the form of a conditional expectation (i.e., a projection on function space), we have recently studied necessary and sufficient conditions under which the projection operator formalism yields an approximation for nonreversible (e.g. driven) systems (Duong et al., 2025). Measuring the distance between the marginal distributions of the resolved variables for the full- and the low-order models, the accuracy of the low-order model can be measured (Hartmann et al., 2020).  

By comparing the low-order stochastic model results with data from the precession experiment, the hope is not only to capture the wave interactions correctly and develop a stochastic extension of the existing amplitude equations, but also to reduce the order of the existing model even further. 

M.H Duong, C. Hartmann, and M. Ottobre, arXiv preprint,  arXiv:2506.14939, 2025.

C. Hartmann, L. Neureither, and U. Sharma, SIAM J. Math. Anal. 52(3), 2689-2733, 2020.

R. Lagrange, P. Meunier, F. Nadal, C Eloy, J. Fluids Mech. 666, 104–145, 2011.

A.J. Majda, I. Tomofeyev, E. Vanden Eijnden, PNAS, 96(26), 14687-14691, 1999.

W. Xu, U. Harlander, Rev. Phys. Fluids., 5(9), 094801-21, 2020.

 

How to cite: Harlander, U. and Hartmann, C.: Low-dimensional stochastic amplitude equations for a precessing rotating cylinder, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5335, https://doi.org/10.5194/egusphere-egu26-5335, 2026.

EGU26-8143 | PICO | NP2.1

Climate Oscillations and Linear Gaussian Nonequilibrium Steady-States 

Jeffrey Weiss, Roberta Benincasa, Dann Du, and Gregory Duane

Climate oscillations such as the El Niño–Southern Oscillation (ENSO) and the Madden–Julien Oscillation (MJO) dominate aspects of climate variability, yet they are often challenging to accurately capture in climate models. Due to their disparate underlying physical processes, any potential commonality between different climate oscillations is obscured. Common underlying dynamics is suggested by the success of relatively low-dimensional linear inverse modeling (LIM). LIMs represent climate oscillations as linear Gaussian nonequilibrium steady states (LG-NESS) defined by stochastic differential equations. Here we develop the theory of LG-NESS’s and compare with observations and models of climate oscillations.

ENSO and the MJO are often described by two-dimensional indices such as the leading SST EOFs for ENSO, or the Realtime Multivariate MJO index. The LIM algorithm parameterizes the dynamics in the index coordinate system as a two-dimensional LG-NESS specified by seven parameters. We decompose the parameter space into four parameters that define the coordinate system of the index, and three parameters that define its intrinsic dynamics. This allows us to transform all 2d LG-NESS’s to a common three-dimensional dynamical parameter space. Coordinate-invariant quantities depend only on the three dynamical parameters, while coordinate-dependent quantities can be transformed back to the original index coordinate system and depend on all seven parameters.

We parameterize ENSO and the MJO in this three-dimensional dynamical parameter space and find that, despite their distinct physical mechanisms and timescales, they lie within a narrow region of parameter space, indicating a similarity in the underlying phase-space dynamics. We compare observed and modeled dynamics with those of their parameterized LG-NESS, evaluating predictability, thermodynamic properties, and event statistics. We find this minimal three-parameter model reproduces many features of climate oscillations, revealing a deep dynamical similarity  among climate oscillations.

 

How to cite: Weiss, J., Benincasa, R., Du, D., and Duane, G.: Climate Oscillations and Linear Gaussian Nonequilibrium Steady-States, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8143, https://doi.org/10.5194/egusphere-egu26-8143, 2026.

EGU26-8761 | ECS | PICO | NP2.1

Whiplash weather in ENSO Transition Years Identified by A Novel Cascading Extremes Index 

Qimin Deng, Louise Slater, Christian Franzke, Yixuan Guo, and Zuntao Fu

Cascading extreme weather events, characterized by sequential occurrences of distinct extremes such as heatwaves, floods or droughts, pose increasing risks in a warming climate. However, existing approaches for identifying such events focus either on temporal persistence or spatial coherence alone, and are thus unable to identify the most severe events with both characteristics. Here, we propose a new approach based in dynamical systems theory that treats variables as coupled systems, with a view to enable their mechanistic understanding. We illustrate the application of the method to temperature and relative humidity data during the period 1979-2020, identifying cascading heat-drought extremes over the Mississippi, southeastern China and France. While these events are controlled by different large-scale climate modes and blocking patterns, nine of the events occurred during rapid transitions (<12 months) from El Niño to La Niña. In China, these transitional events were consistently preceded by heavy rainfall approximately two weeks earlier. Key drivers include the prolonged presence of the western north Pacific subtropical high and land-atmosphere feedbacks. Our findings uncover the speed and severity of cascading wet-dry transitions within as little as two weeks during El Niño transition years, and the need for a greater understanding of their driving mechanisms.

How to cite: Deng, Q., Slater, L., Franzke, C., Guo, Y., and Fu, Z.: Whiplash weather in ENSO Transition Years Identified by A Novel Cascading Extremes Index, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8761, https://doi.org/10.5194/egusphere-egu26-8761, 2026.

EGU26-10698 | PICO | NP2.1

Evaluation of CMIP6 Models in Simulating Network-Based Early Warning Signals of El Niño 

Naiming Yuan, Jiangxue Han, and Josef Ludescher

Network-based early warning signals of El Niño have been recognized for more than a decade, however, it remains unclear whether current climate models can reproduce these signals. Here, we evaluate simulations from both the pre-industrial control and historical experiments of CMIP6 models. While none of the models exhibited skill in either experiment, performance was generally better in the historical runs, suggesting that the inclusion of external forcing may improve model simulations of the early warning signals. Further analysis indicates that some models such as CESM2, FGOALS-g3, and MRI-ESM2-0 may provide potentially useful early warning information for El Niño events, but their warning signals tended to emerge later than those in reanalysis data. Using a new network-based evaluation metric to assess air-sea interactions in the tropical Pacific, we find that model performance in simulating early warning signals is generally linked to their ability to simulate these interactions. This highlights the importance of improving representations of air-sea coupling in current models. For future investigations into the physical mechanisms underlying the network-based early warning signals, CESM2, FGOALS-g3, and MRI-ESM2-0 are recommended due to their relatively better performance compared to the other models considered in this work, although the causes of their delayed signal emergence require further exploration.

How to cite: Yuan, N., Han, J., and Ludescher, J.: Evaluation of CMIP6 Models in Simulating Network-Based Early Warning Signals of El Niño, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10698, https://doi.org/10.5194/egusphere-egu26-10698, 2026.

The growing availability of multiple operational ocean data services provides unprecedented opportunities for applications such as environmental incident response, search and rescue operations, and maritime management. At the same time, despite their widespread use, most ocean datasets offer limited information regarding their performance and consistency with real-world observations.

In this presentation, I address this gap by introducing a methodology to assess uncertainty in ocean transport predictions derived from different ocean data products. Building on recent work that links transport uncertainty—understood here as deviations from ground truth—to invariant dynamical structures in the ocean [1–3], the proposed approach, discussed in [4], exploits these links to guide statistical averaging strategies. We examine how well model-predicted material transport aligns with observational evidence across different dynamical scales, including scales above the mesoscale, the mesoscale, and the submesoscale. This perspective provides a systematic pathway for quantifying the performance of different data sources and assessing their overall quality and reliability.

References:

[1] G. García-Sánchez, A. M. Mancho, A. G. Ramos, J. Coca, B. Pérez-Gómez, E. Alvarez-Fanjul, M. G. Sotillo, M. García-León, V. J. García-Garrido, S. Wiggins. Very High Resolution Tools for the Monitoring and Assessment of Environmental Hazards in Coastal Areas. Frontiers in Marine 7, 605804 (2021).

[2] G. García-Sánchez, A. M. Mancho, S. Wiggins. A bridge between invariant dynamical structures and uncertainty quantification. Commun. Nonlinear Sci. Numer. Simul. 104, 106016 (2022).

[3] G. García-Sánchez, A. M. Mancho, M. Agaoglou, S. Wiggins. New links between invariant dynamical structures and uncertainty quantification. Physica D 453 133826 (2023).

[4] G. García-Sánchez, M. Agaoglou, E.M.C Smith, A. M. Mancho. A Lagrangian uncertainty quantification approach to validate ocean model datasets. Physica D 475 134690 (2025).

Acknowledgments:

Support from PIE project Ref. 202250E001 funded by CSIC, from grant PID2021-123348OB-I00 funded by MCIN/ AEI /10.13039/501100011033/ and by FEDER A way for making Europe.

How to cite: Mancho, A. M.: Understanding Uncertainty in Ocean Transport Inferred from Multiple Data Sources, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13663, https://doi.org/10.5194/egusphere-egu26-13663, 2026.

EGU26-15454 | PICO | NP2.1

A Cellular Automata Model of Tropical Oceanic Rain Clusters with Self-organized Criticality 

Kevin Cheung, Chee-Kiat Teo, and Tieh-Yong Koh

Tropical oceanic rain clusters exhibit complex organization patterns that can reveal fundamental principles governing convective systems. In this study, we develop a simple cellular automaton (CA) model that captures essential dynamics of tropical convection, using only a minimal set of physical rules. The model focuses on how local destabilization and stabilizing feedbacks, mediated by gravity waves, shape the spatial structure of rain clusters. Specifically, the distributions of the cluster area, A, and total rain rate, R, for tropical oceanic rain clusters from the CA model are analyzed for their scaling exponent ζA, ζR, and β where ; f(s) the probability distribution of S, E(R¦a) ~ aβ, E(R¦a) the conditional expectation of R given A = a.

We find that the CA naturally exhibits critical behavior, resembling patterns seen in percolation theory. Specifically, the size distribution of rain clusters follows a scaling law whose exponent is remarkably robust and closely matches the theoretical value for 2D percolation. This suggests that rain clusters in certain tropical regions may organize in a “percolation-like” manner, where large, connected clusters emerge in a critical state. Comparisons with regional climate model simulations over the tropics (Teo et al. 2021) show that rain clusters over the Indian Ocean and tropical Atlantic behave similarly to the critical clusters in our CA, while deviations over the Pacific may result from stronger large-scale destabilization over the western Pacific warm pool and the eastern Pacific ITCZ. Although our CA reproduces key scaling relationships between cluster area and rain rate, it does not fully account for the observed ζA ~ 5/3 reported in observational studies (Teo et al. 2017). We propose a simplified version of the CA that may reconcile this difference through tunable criticality.

References:

Teo, C.-K., H.-N. Nuynh, T.-Y. Koh, K. K. W. Cheung, B. Legras, L.-Y. Chew, and L. Norford, 2017: The universal scaling characteristics of tropical oceanic rain clusters. J. Geophys. Res. Atmos., 122, 5582–5599, https://doi.org/10.1002/2016JD025921.

Teo, C.-K., T.-Y. Koh, K. K. W. Cheung, B. Legras, H. Nguyen, L.-Y. Chew, and L. Norford, 2021: Scaling characteristics of modeled tropical oceanic rain clusters. Quart. J. Roy. Meteorol. Soc., 147, 1055–1069, https://doi.org/10.1002/qj.3959.

How to cite: Cheung, K., Teo, C.-K., and Koh, T.-Y.: A Cellular Automata Model of Tropical Oceanic Rain Clusters with Self-organized Criticality, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15454, https://doi.org/10.5194/egusphere-egu26-15454, 2026.

While understanding systemic risk in complex systems has gained growing attention, less effort is often dedicated to understanding the system itself.  Particularly, the typology of complex systems and collapse mechanisms that are consistent across domains remains understudied. Hence, critical questions arise, such as what do we need to know about the system’s characteristics to predict systemwide collapse, identify leverage points, or design resilience interventions? What system properties allow knowledge gained from one system to be generalized to other taxonomically similar systems? What signals can be deduced from a few systems’ global parameters to determine whether a system is in a stable, unstable, or critical region of its adjacent becoming?"

 

Answering these questions requires determining the typology of complex systems, which enables the study of system-level behaviors independently of the specific details of individual agents. This leads to universality, facilitating the study of collapse mechanisms transferable to other typologically similar systems, thereby providing insight into systemic risk.

 

This presentation introduces a novel typology of complex systems based on the concept of “adjacent becoming,” drawing on works of Stuart Kaufmann, C.S. Holling, and Marten Scheffer, among others which have established the language of attractors, regime shifts, evolution, and panarchical resilience in complex systems. The System’s Adjacent Becoming (SAB) is what the system is positioned to become while appearing to be in a stable condition, i.e., potential for a critical transition in deep stability. Such a proximal transformation potential can be characterized by four interrelated components consisting of a) the system's location in phase space and proximity to the most accessible alternative attractors, b) the topography of the current boundary basin, c) the system's current momentum and energy state, and d) the prospective trajectory and regime that a transition to a given alternative attractor would induce. These four components collectively determine the SAB potential, and thus the likelihood and qualitative characteristics of an imminent regime shift.

 

To assess SAB, what system has, what system does, and what system could become are the critical questions.  For such an assessment, a SAB-informed typology would be the first step. Therefore, the four SAB components lead to types based on nine interconnected system variables: (1) micro-macro dynamic type; (2) state of information processing and memory capacity; (3) degree of teleonomic coherence across levels and panarchical organization; (4) degree of agent heterogeneity; (5) type and intensity of emergence; (6) functional and computational efficiency rate; (7) initial condition and presence of path dependency; (8) manifestation of critical slowing down indicators and bifurcation proximity signals and (9) the existing geometric attractor landscape. 

This SAB-informed typology is phenomenologic-mechanistic in nature, which helps to learn about the structural and dynamical signatures of critical transitions and the quality of the new becoming, offering a unified language for understanding how complex adaptive systems of any kind approach their adjacent becoming and what determines whether they persist, transform, or collapse. This framework remains theoretical with operationalization challenges; future work must advance toward measurable proxies for the nine categories to quantify SAB of real-world systems.

How to cite: Zamanifar, M. and Samaro, N.: Systemic risk in complex systems: understanding the system based on the system’s adjacent becoming, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21170, https://doi.org/10.5194/egusphere-egu26-21170, 2026.

EGU26-2241 | Orals | AS1.20

Seasonal Rossby Wave Dynamics Driving Winter and Summer Temperature Extremes in the Arabian Peninsula 

Jiya Albert, Mariam Fathima Navaz, Abdul Azeez Saleem, Venkata Sai Chaitanya Akurathi, Salim Lateef, Muhammad Shafeeque, and Luai Alhems

Atmospheric Rossby waves exert a strong control on the emerging pattern of summer heat and winter cold over the Arabian Peninsula, yet their regional impacts remain poorly quantified. This study uses 25 years (2000–2024) of reanalysis and observational data to assess how upper-tropospheric Rossby wave activity modulates seasonal 2 m temperature extremes over Saudi Arabia and how these responses are embedded in large-scale teleconnections linked to ENSO and Indo-Pacific variability. The analysis focuses on the evolution of warm-core structures in summer, the spatial spread of winter cold anomalies, and two recent extreme years, 2017 and 2023, that reveal the sensitivity of the Peninsula to Rossby wave regime shifts.

Results show a progressive amplification and spatial expansion of August near-surface temperatures across Saudi Arabia, with the 37–38 °C isotherms migrating northward and westward after 2010 to form a quasi-continuous warm core spanning the eastern lowlands, Rub al Khali, and central plateau. The fraction of land exceeding 39 °C in August increased from isolated spots in the early 2000s to over 20% after 2015, signifying a step-like intensification of summertime heat. Composite analyses indicate that these hot cores coincide with upper-level anticyclonic ridges and subsidence maxima, consistent with Rossby wave–induced adiabatic warming and suppressed convection.

Within this long-term warming context, 2017 stands out as a dynamical outlier. Amplified and breaking Rossby waves over the Middle East generated a quasi-stationary ridge over the Peninsula, producing exceptionally broad August heat with mean temperatures above 38 °C across central and northeastern regions. In winter 2017, enhanced wave activity drove deep trough intrusions and widespread sub‑16 °C anomalies, yielding an unusual combination of extreme summer heat and pronounced winter cooling within one year. A renewed Rossby forcing episode in 2023 accompanied one of the hottest summers on record, when the southeastern warm core intensified and spread northwestward while winter again featured strong meridional temperature gradients and broad cold coverage.

Wave activity flux diagnostics and teleconnection analyses reveal that both 2017 and 2023 extremes arose from Indo-Pacific–Eurasian Rossby wave trains. In 2017, La Niña–like conditions and a positive Indian Ocean Dipole excited a Eurasian wave train that channelled energy along the subtropical jet, reinforcing anticyclonic ridging in summer and deep winter troughs. In 2023, an ENSO phase transition under neutral IOD conditions triggered renewed Rossby dispersion from the tropical western Pacific into the Asian jet, again focusing anomalous ridging and subsidence over the Peninsula.

These results suggest that modest upstream anomalies now yield amplified regional thermal responses, implying increased dynamical gain due to background warming and altered land–atmosphere coupling. The findings point to a Rossby wave–dominated regime shift since 2017, wherein upper-level wave geometry and teleconnections increasingly control the extent of summer heat and winter cold. Saudi Arabia thus emerges as a dynamically sensitive node in the global Rossby waveguide system.

How to cite: Albert, J., Navaz, M. F., Saleem, A. A., Chaitanya Akurathi, V. S., Lateef, S., Shafeeque, M., and Alhems, L.: Seasonal Rossby Wave Dynamics Driving Winter and Summer Temperature Extremes in the Arabian Peninsula, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2241, https://doi.org/10.5194/egusphere-egu26-2241, 2026.

Atmospheric blocking, conventionally studied as a quasi-stationary phenomenon, often exhibits zonal movement under the influence of factors like the background flow and retrograding Rossby waves. However, the impact of this mobility on cold extremes remains under-investigated. This study classifies atmospheric blocking events during the winters of 1979/80–2020/21 into westward-moving, eastward-moving, and quasi-stationary types to analyze their distinct impacts on surface air temperature by region.

Our results show that westward-moving blocks occurred most frequently over the western North Pacific, whereas quasi-stationary blocks were dominant in most other regions. In terms of duration, westward-moving blocks consistently persisted longer than the other types across all regions. Notably, these long-lasting, westward-moving events were closely associated with inducing strong cold waves in downstream areas during their dissipation phase. This is attributed to the enhanced advection of cold Arctic air by blocking-induced low-level wind anomalies. These characteristics were successfully reproduced in CESM1-LENS simulations, suggesting that a better understanding of blocking mobility can contribute to improving extreme cold surge prediction.

How to cite: Kim, S.-H. and Kim, B.-M.: Characterizing Blocking Mobility and Its Role in Northern Hemisphere Cold Extremes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2300, https://doi.org/10.5194/egusphere-egu26-2300, 2026.

EGU26-2413 | ECS | Posters on site | AS1.20

On the interpretation of the pressure vertical velocity 

Juntian Chen, Sergiy Vasylkevych, Nedjeljka Žagar, and Cathy Hohenegger

Pressure vertical velocity (ω = Dp/Dt) is commonly approximated from the geometric vertical velocity (w = Dz/Dt) as ω ≈ -ρgw, which invokes the hydrostatic relation ∂p/∂z ≈ -ρg together with the additional assumption that local pressure tendency and horizontal pressure advection term are negligible at planetary and synoptic scales. Using global nonhydrostatic simulations with the ICON model, we show that the horizontal pressure advection term can be relatively large compared with the vertical pressure advection term at planetary-to-synoptic scales in regions of strong jets such as in the winter stratosphere, contradicting the conventional assumption ω ≈ -ρgw. We further show that the horizontal and vertical pressure advection terms exhibit a predominantly out-of-phase structure and that their comparable amplitudes lead to substantial cancellation. As a consequence, ω can be suppressed or amplified at large scales relative to the -ρgw diagnostic, despite the validity of the hydrostatic balance. Scale diagnostics indicate that the large-scale enhancement of the horizontal pressure advection arises from interactions between the mean flow and eddies. From an energetic perspective, these advection terms correspond to compensating contributions of pressure-gradient work in different directions. Consequently, ω behaves more like the net pressure gradient work, rather than a direct measure of vertical motion.

How to cite: Chen, J., Vasylkevych, S., Žagar, N., and Hohenegger, C.: On the interpretation of the pressure vertical velocity, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2413, https://doi.org/10.5194/egusphere-egu26-2413, 2026.

EGU26-2487 | Orals | AS1.20

The evolution of cyclonic and anticyclonic Rossby wave breaking morphologies and their importance in extremes 

Michael A. Barnes, Michael J. Reeder, and Thando Ndarana
Rossby waves are fundamental meteorological phenomena in the extratropics. When these waves amplify and break, they often lead to extreme weather events, including heatwaves, heavy rainfall, and strong winds. Here we apply an objective classification method to identify equatorward anticyclonic and cyclonic Rossby wave breaking morphologies, analogous to the LC1 and LC2 types identified in previous research. Anticyclonic Rossby wave breaking zones are shown to evolve as expected, representing the barotropic decay of baroclinic Rossby wave packet. Composite analysis of the evolution of cyclonic Rossby wave breaking morphologies however shows that these morphologies develop from the debris of preceding anticyclonic Rossby wave breaking. Cyclonic morphologies are further linked to Rossby wave packet generation and downstream development. The role of Rossby wave breaking in extreme weather is illustrated through the example of heavy rainfall along Australia’s east coast, emphasizing its importance in the generation of such extremes.

How to cite: Barnes, M. A., Reeder, M. J., and Ndarana, T.: The evolution of cyclonic and anticyclonic Rossby wave breaking morphologies and their importance in extremes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2487, https://doi.org/10.5194/egusphere-egu26-2487, 2026.

EGU26-2492 | ECS | Posters on site | AS1.20

The Influence of Tropopause Potential Vorticity Circulation Forcing on the Development of the East Asian Cold Wave in December 2023 

Yanxi Li, Guoxiong Wu, Yimin Liu, Bian He, Jiangyu Mao, and Chen Sheng

In December 14 to 16, 2023, East Asia experienced a severe cold wave, with record-breaking low temperatures and consequently severe natural disasters over broad areas. Results suggest that anomalous downward potential vorticity circulation (PVC) forcing across the tropopause played a critical role in triggering and amplifying this event. The results indicated that in early December, a strong positive potential vorticity substance (PVS) reservoir accompanied by an anomalous downward PVC persisted in the lower stratosphere over Siberia, whereas two distinct upper tropospheric fronts (UTFs) were located over East Asia. By December 12, as the downward PVC penetrated the tropopause into the troposphere, enhancing the northern UTF and triggering a perturbation trough at its western end. This northern trough propagated faster eastward along the UTF than its southern counterpart, and its PVS was intensified by the descending northerly flow. As the two UTFs merged on the eastern Tibetan Plateau, the northern trough was phase-locked with the southern trough, forming a deep East Asian trough with a well-developed PVS. The prominent cold descending northerly flow dominated the troposphere behind the trough, generating extremely high surface pressure and abnormal cold temperature advection below. Consequently, a severe cold wave swept over East Asia. This study improves upon previous work by directly linking tropopause PVC forcing to trough phase-locking, a previously overlooked pathway for cold wave amplification.

How to cite: Li, Y., Wu, G., Liu, Y., He, B., Mao, J., and Sheng, C.: The Influence of Tropopause Potential Vorticity Circulation Forcing on the Development of the East Asian Cold Wave in December 2023, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2492, https://doi.org/10.5194/egusphere-egu26-2492, 2026.

EGU26-2689 | ECS | Orals | AS1.20

Resolution Sensitivity of Rossby Wave Breaking and Warm Conveyor Belts in Global ICON Simulations 

Marius Rixen, Andreas Prein, Praveen Pothapakula, Michael Sprenger, and Christian Zeman

Forecast busts over Europe—periods of abnormally low predictive skill—are often associated with extreme weather events and linked to misrepresented upper-level dynamics, including latent heating from mesoscale convective systems (MCSs), Rossby wave breaking, and warm conveyor belt (WCB) outflow. This study investigates how explicitly resolving mesoscale processes affects the simulation of these key mechanisms in global ICON ensemble forecasts at grid spacings ranging from 40 km down to 2.5 km. As a test case, we analyze a forecast bust from ECMWF’s Integrated Forecasting System (IFS) related to the development of Storm Dennis (February 2020), the second-most intense North Atlantic winter storm of the past 150 years, and compare ICON with IFS.

We find a systematic improvement in forecast skill with finer grid spacing. Coarse-resolution simulations reproduce the forecast bust and fail to capture the correct trough–ridge pattern, while convection-permitting simulations more accurately represent upper-level potential vorticity anomalies, WCB structure, and cyclone development.

Our analysis reveals a multi-stage chain of error growth arising from several interacting factors. Large initial-condition uncertainties over the North Pacific provide a background sensitivity, but the strongest early error growth occurs over the central United States, coinciding with a period of deep convection from MCSs. Convection-permitting simulations produce stronger and more coherent MCSs, leading to enhanced negative PV injection near 250 hPa and substantially reduced Rossby wave activity errors. In contrast, coarser-resolution simulations exhibit weaker or misplaced MCSs, resulting in larger errors in the upper-tropospheric flow. These midlatitude convective differences subsequently modulate the intensity and orientation of downstream WCBs over the North Atlantic. The WCB then amplifies the pre-existing errors, linking the central-U.S. convective phase to the eventual European forecast bust.

Overall, our results demonstrate that mesoscale processes over North America—especially MCS-driven PV perturbations—play a key role in setting the predictability of the North Atlantic flow regime during Storm Dennis. Convection-permitting global simulations improve the representation of these processes and offer a physically consistent pathway toward reducing forecast busts in high-impact weather situations. To assess the robustness and generality of these findings, additional case studies are currently being analyzed.

How to cite: Rixen, M., Prein, A., Pothapakula, P., Sprenger, M., and Zeman, C.: Resolution Sensitivity of Rossby Wave Breaking and Warm Conveyor Belts in Global ICON Simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2689, https://doi.org/10.5194/egusphere-egu26-2689, 2026.

EGU26-2944 | Orals | AS1.20

The maintenance of a zonally asymmetric subtropical jet 

Orli Lachmy and Ian White

The subtropical jet dominates over specific longitudinal sectors during both winters. The major source of this zonal asymmetry is localized tropical convection. In particular, during austral winter, the wide and powerful convection over the Asian monsoon region and Maritime Continent drives a subtropical jet over the Indian Ocean, Australia and the west and central Pacific. Further downstream in the east Pacific the jet tilts poleward, gradually shifting towards eddy-driven jet characteristics, while in the Atlantic sector only an eddy-driven jet prevails.

In this study, we show that the upper tropospheric circulation pattern over the whole Southern Hemisphere during winter is similar to that in an idealized model simulation, where the only zonal asymmetry source is localized tropical convection in the summer hemisphere. A similar momentum budget is found for the observations and model simulation. The first-order momentum balance is the geostrophic balance associated with a stationary Rossby wave driven by tropical convection. The upstream part of the subtropical jet (the Indian Ocean jet) is associated with a high equatorward of it, and the downstream part (the Pacific jet) is associated with a low poleward of it. This demonstrates that the subtropical jet zonally asymmetric component is a manifestation of a stationary Rossby wave in the upper troposphere. The second-order momentum balance is associated with approximate absolute angular momentum conservation in the localized Hadley cell, as is the dominant balance in zonally symmetric models. The third-order momentum balance is between meridional advection of absolute angular momentum and zonal momentum advection. Transient eddy momentum fluxes are negligible in the maintenance of the subtropical jet zonal structure.

How to cite: Lachmy, O. and White, I.: The maintenance of a zonally asymmetric subtropical jet, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2944, https://doi.org/10.5194/egusphere-egu26-2944, 2026.

EGU26-3038 | ECS | Posters on site | AS1.20

Quantifying the influence of Barents-Kara sea ice loss on Ural blocking 

Ernest Agyemang-Oko and Marlene Kretschmer

Arctic amplification has been linked to significant changes in mid-latitude weather patterns, including the increasing frequency and persistence of extreme weather events. This study investigates the influence of Barents-Kara (BK) sea-ice variability on wintertime Ural blocking and its role in Eurasian cold temperature anomalies. Using ERA5 reanalysis data, we analyse Ural blocking frequency and persistence based on two commonly used blocking indices (an absolute geopotential height reversal index and an anomaly-based index method). The relationships between BK sea ice, Ural blocking, and Eurasian surface temperature are examined within a causal network framework, accounting for ENSO as a potential common driver by including it as a covariate and by stratifying the analysis by ENSO phase. We find that Ural blocking events occur more frequently and persist longer during winters with reduced BK sea ice. Although, results are sensitive to blocking index but remain qualitatively consistent and robust across indices. Composite analyses show a characteristic warm-Arctic/cold-Eurasia temperature pattern during Ural blocking events, which is amplified during winters with low BK sea ice and La Niña conditions. To assess whether Ural blocking is influenced by specific Arctic background conditions, we further classify winters into Deep and Shallow Arctic warming regimes over the Barents-Kara region. We find that Ural blocking occurs more frequently and is more persistent under Deep Arctic warming states, leading to a stronger cold-Eurasia temperature response compared to Shallow warming regimes. By statistically quantifying the relationships between Arctic sea ice, Ural blocking, and Eurasian temperature variability, this work advances the understanding of Arctic-midlatitude interactions.

Keywords: Arctic Amplification, Ural blocking, Barents-Kara sea ice, ENSO, Blocking indices, Blocking frequency and persistence, Eurasian cold winters.

How to cite: Agyemang-Oko, E. and Kretschmer, M.: Quantifying the influence of Barents-Kara sea ice loss on Ural blocking, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3038, https://doi.org/10.5194/egusphere-egu26-3038, 2026.

EGU26-3695 | ECS | Posters on site | AS1.20

The importance of polar and singular waveguides for the occurrence of Rossby wave resonance 

Tobias Hempel and Volkmar Wirth

The occurrence of extreme weather has recently been associated with the mechanism of Rossby wave resonance along a circumglobal jet. Resonance is possible to the extent that the jet acts as a zonal waveguide. Recently, a method was introduced to diagnose this mechanism in the framework of the linear barotropic model through numerically solving a judiciously designed model configuration. In that method, any wave activity leaving the jet region is dissipated in sponges and, hence, discarded from further consideration.

The present work goes a step further by explicitly accounting for polar and singular waveguides, which occur through wave reflection off the pole or off a critical level. In the absence of damping, these reflective boundaries generate additional resonant cavities and allow higher meridional modes to participate in the resonance. These higher meridional modes imply resonance at multiple zonal wavenumbers, in stark contrast with the earlier results. However, when a small amount of damping is included, any wave activity is strongly dissipated before these reflecting surfaces are encountered. Consequently, the impact of the polar and the singular waveguides vanishes, and the resonant behavior reduces to that from the original diagnostic. It is concluded that the impact of reflecting surfaces beyond the jet region proper is unlikely to be of practical importance for diagnosing the Rossby wave resonance along a circumglobal midlatitude jet.

How to cite: Hempel, T. and Wirth, V.: The importance of polar and singular waveguides for the occurrence of Rossby wave resonance, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3695, https://doi.org/10.5194/egusphere-egu26-3695, 2026.

EGU26-4663 | Posters on site | AS1.20

Interdecadal changes and the role of Philippine Sea convection in the intensification of Indian spring heatwaves 

Jung Ok, Eun-Ji Song, Sinil Yang, Baek-Min Kim, and Ki-Young Kim

Severe heatwaves have become increasingly frequent over the Indian subcontinent in recent decades. This study found that the increase in extreme heatwaves is related to a significant decadal change in surface temperatures over the Indian subcontinent, and revealed that the increase in convective activity in the Philippine Sea plays a crucial role in this decadal change in surface temperature. Specifically, the surface temperature over the Indian subcontinent in spring has increased significantly by approximately 0.64 ◦C in recent years (1998–2022: post-1998) compared to the past (1959–1997: pre-1998), leading to more intense and frequent heatwaves, particularly in March and April. The difference in atmospheric changes between these two periods shows that the enhancement of convective activity over the Philippine Sea drives an anomalous elongated anticyclonic circulation over the Indian subcontinent. This circulation pattern, marked by clearer skies and increased incident solar radiation, significantly contributes to the heat extremes in the Indian subcontinent. Additionally, stationary wave model experiments demonstrate that local diabatic heating over the Philippine Sea is significantly linked to robust spring Indian heatwaves through the Matsuno–Gill response.

How to cite: Ok, J., Song, E.-J., Yang, S., Kim, B.-M., and Kim, K.-Y.: Interdecadal changes and the role of Philippine Sea convection in the intensification of Indian spring heatwaves, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4663, https://doi.org/10.5194/egusphere-egu26-4663, 2026.

Atmospheric Rossby waves are a fundamental component of large-scale circulation and low-frequency atmospheric variability. In classical theory, quasi-stationary planetary waves are characterized by infinite periods and are typically regarded as slowly varying background disturbances, which limits their ability to explain the widespread intraseasonal oscillations (ISOs) observed in the atmosphere. Given that ISOs share comparable spatial and temporal scales with planetary waves, a nonstationary Rossby waves framework provides a promising theoretical basis for interpreting their propagation characteristics.

In this study, we develop a theoretical framework for nonstationary horizontally propagating Rossby waves embedded in a prescribed background flow. We systematically derive the necessary conditions for the existence of three propagating solution branches, expressed equivalently in terms of the supremum and infimum of phase speed and wave period. Both the phase-speed and period supremum and infimum are determined by the background wind field, while the supremum and infimum of the period additionally depend on the zonal wavenumber. Two distinct regimes of admissible phase-speed and period ranges emerge, reflecting different background-flow configurations.

By combining these theoretical constraints with atmospheric reanalysis data, we diagnose the climatological supremum and infimum of nonstationary Rossby wave speriods in both the upper and lower troposphere over key tropical regions. The results reveal pronounced seasonal and regional variations in the theoretical period ranges due to differences in background circulation between tropospheric layers. In the upper troposphere, the equatorial Indian–western Pacific region does not support eastward-propagating solutions, whereas in the lower troposphere, eastward-propagating nonstationary waves with intraseasonal periods become possible under monsoonal flow conditions, consistent with monsoon ISO characteristics. During boreal winter and spring, the theoretical period supremum and infimum of lower-tropospheric nonstationary waves over the equatorial Indian–western Pacific exhibit Madden–Julian Oscillation (MJO)-like features. Over the equatorial Atlantic, vertically asymmetric background flows lead to distinct propagation characteristics between the upper and lower troposphere, consistent with observed ISO structures.

This work extends the classical theory of Rossby waves propagation by incorporating nonstationary waves and provides a unified theoretical interpretation linking nonstationary planetary waves to tropical intraseasonal variability.

How to cite: Liu, Y. and Li, J.: The theory and climatological characteristics of nonstationary horizontally Rossby waves, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4697, https://doi.org/10.5194/egusphere-egu26-4697, 2026.

EGU26-5587 | ECS | Posters on site | AS1.20

The role of diabatic heating in Rossby wave breaking 

Marc Federer, Mona Bukenberger, and Talia Tamarin-Brodsky

Rossby wave breaking (RWB) is a key process through which synoptic-scale eddies reorganize the extratropical circulation, interacting with jet shifts, storm track variability, and the persistence of weather regimes. Despite extensive evidence that diabatic heating strongly influences synoptic eddies and supports blocking, its influence on when and how Rossby waves break remains largely unexplored. This gap limits our physical understanding of how moist processes reshape the potential vorticity structure that governs RWB and, in turn, the large-scale circulation.

We investigate the influence of diabatic processes on RWB using aquaplanet simulations at 100, 20, and 2.5 km horizontal resolution, which systematically alter the representation of diabatic heating. By comparing RWB frequency, geometry, and life cycles across resolutions, we isolate how the resolution-dependent representation of diabatic heating shapes RWB and the RWB-mediated circulation response, including jet latitude and storm track position. These idealized results are complemented by an observational analysis of RWB events and associated warm conveyor belts in ERA5 reanalyses.

Together, these analyses provide new physical insight into how diabatic processes modulate RWB and thereby shape the extratropical circulation, with implications for the interpretation of resolution-dependent circulation biases and the representation of moist processes in weather and climate models.



How to cite: Federer, M., Bukenberger, M., and Tamarin-Brodsky, T.: The role of diabatic heating in Rossby wave breaking, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5587, https://doi.org/10.5194/egusphere-egu26-5587, 2026.

EGU26-6203 | ECS | Posters on site | AS1.20

MJO modulation on the cold extreme over the North America in a recent decade 

Minju Kim, Hyemi Kim, and Mi-kyung Sung

Over the last decade, North American cold extreme events have exhibited a notable shift in timing, occurring more frequently in February rather than earlier in winter. This delayed-season tendency suggests a strong influence from intraseasonal climate variability. In addition we identify a pronounced warming trend in sea surface temperature (SST) over the equatorial Pacific warm pool region, with the warming signal becoming particularly distinct during the most recent decade. We examine a dynamical linkage between the Madden-Julian Oscillation (MJO) and cold extremes over the North America in late-winter. As the equatorial Pacific warm pool region shows a warming trend, the eastward propagation speed of the MJO tends to slow, resulting in increased residence time and a higher occurrence frequency of MJO phase 7 during February for a recent decade. Under these conditions, persistent convection over the equatorial western Pacific enhances diabatic heating and strengthens tropical thermal forcing. This sustained forcing excites Rossby wave responses, facilitating downstream wave propagation into the central North America region. The resulting MJO teleconnections favor the development of large-scale flow patterns conducive to cold extremes over North America, thereby increasing the likelihood of February cold waves.

How to cite: Kim, M., Kim, H., and Sung, M.: MJO modulation on the cold extreme over the North America in a recent decade, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6203, https://doi.org/10.5194/egusphere-egu26-6203, 2026.

EGU26-6324 | Orals | AS1.20

Uncovering Missing Eurasian Blocking Events and Their Robust Role in East Asian Winter Extremes 

Baek-Min Kim, Hayeon Noh, Ho-Young Ku, and Mi-Kyung Sung

Despite the profound influence of Eurasian blocking on the East Asian winter monsoon, its objective detection remains a challenge due to a systematic under-detection in standard algorithms. The widely adopted Hybrid method (HYB) applies a hemispheric constant threshold for anomaly detection prior to the flow reversal criterion. This constrained design neglects the lower geopotential height variability characteristic of the Eurasian continent, resulting in the premature filtering of meteorologically significant events. Here, we propose the Regional Hybrid method (RHYB), a refined framework that incorporates anomaly thresholds tailored to local geopotential height variance. By reconciling detection criteria with regional physical characteristics, RHYB explicitly captures "reversal-dominated" systems—events with clear flow disruption but modest amplitude—that were previously obscured. Using ERA5 reanalysis, we demonstrate that these newly identified events are robust drivers of severe wintertime cold surges over East Asia, indicating that their prior omission has led to a significant underestimation of regional climate risks. These results underscore that RHYB is an essential tool for accurately diagnosing midlatitude extremes and their evolving dynamics in a warming world.

How to cite: Kim, B.-M., Noh, H., Ku, H.-Y., and Sung, M.-K.: Uncovering Missing Eurasian Blocking Events and Their Robust Role in East Asian Winter Extremes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6324, https://doi.org/10.5194/egusphere-egu26-6324, 2026.

During April-May 2024, South China experienced an unprecedented extreme precipitation event, leading to substantial socioeconomic losses and human casualties. The primary driver of this event was an exceptionally strong moisture convergence linked to a local low-level horizontal trough. This trough was passively induced by two meridionally-oriented anomalous anticyclones located over the tropical western North Pacific and Northeast Asia. The tropical anticyclone facilitated the advection of abundant moisture towards southern China, while the Northeast Asian anticyclone impeded northward moisture export, jointly resulting in the observed extreme precipitation. The tropical anticyclone represents a typical Kelvin wave response to convection anomalies over the tropical Indian Ocean, which were forced by localized positive sea surface temperature (SST) anomalies. In contrast, the Northeast Asian anticyclone was a node of a mid-to-high latitude barotropic Rossby wave train. This Rossby wave train, initiated by the tropical Atlantic convection, was guided towards Northeast Asia by a transient eddy-driven polar front jet. Although the European Centre for Medium-Range Weather Forecasts showed high skill in predicting tropical Atlantic and Indian Ocean SST and associated convection anomalies, its ability to predict the April-May 2024 South China precipitation extreme was limited, primarily owing to difficulties in accurately predicting the strength of polar front jet. Overall, this study highlights the critical role of extratropical mean flow in modulating climate extremes that are responsive to tropical forcing.

How to cite: Liu, X. and Zhu, Z.: A manipulator of the extreme precipitation in South China behind the tropical sea surface temperature: the polar front jet, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6369, https://doi.org/10.5194/egusphere-egu26-6369, 2026.

The mid-latitude jet streams play a defining role in shaping regional weather and climate, making it crucial to understand their current state as well as future changes under anthropogenic forcing. While model uncertainties have reduced over time, significant spread in projections still exists. The problem is exacerbated by a multitude of different jet stream drivers whose influence varies with season and region. This talk will discuss some work in trying to constrain future jet projections and give an overview of regional and seasonal characteristics of jet streams and their drivers. It will further discuss potential new avenues for establishing meaningful physical relationships within the high-dimensional frameworks of jet streams and drivers to better understand regional impacts.

How to cite: Breul, P.: Seasonal and regional jet stream changes, their drivers, and how to connect them., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6800, https://doi.org/10.5194/egusphere-egu26-6800, 2026.

EGU26-7081 | ECS | Orals | AS1.20

Idealized shallow-water simulations of potential vorticity perturbations in zonal jet-waveguides and links to observed dynamical processes 

Vishnupriya Selvakumar, Michael Sprenger, Hanna Joos, and Heini Wernli

This study investigates the propagation of negative potential vorticity (PV) anomalies in idealized shallow-water simulations, with particular emphasis on how their evolution is governed by the structure and latitude of the jet. The initial conditions of the experiments constitute a zonally symmetric midlatitude jet representing a Rossby waveguide, and an isolated, axisymmetric negative PV vortex representing upper-level ridges and diabatically generated outflows associated with warm conveyor belts (WCBs).

The experiments provide a first systematic demonstration that vortex propagation is governed by the combined effects of intrinsic Rossby-wave propagation and advection by the jet, with the relative importance of these processes determined by the latitude of vortex initialization relative to the jet. Importantly, the resulting propagation behavior is not symmetric about the position of the vortex relative to the jet axis. 

These results also provide a direct dynamical analogue for the behavior of WCB outflows across different interaction types with the Rossby waveguide in the real atmosphere. In particular, vortices initiated close to the jet core or slightly equatorward correspond to no-interaction WCB outflows, which exhibit rapid advection and equatorward displacement. The ridge-interaction outflows, characterized by relatively weaker advection, are represented by vortices initialized on the poleward flank of the jet. In contrast, anomalies initialized farther poleward of the jet, with minimal direct influence from the westerlies and quasi-stationary behavior, correspond to blocking and cutoff interactions of WCB outflows.

The structure of the jet is equally important: variations in jet strength in the idealized simulations modulate the degree of eastward advection of the vortices, while changes in jet width and latitude primarily shift the spatial extent of the jet’s influence; in all cases, vortex behavior is governed by its relative position with respect to the Rossby waveguide.

How to cite: Selvakumar, V., Sprenger, M., Joos, H., and Wernli, H.: Idealized shallow-water simulations of potential vorticity perturbations in zonal jet-waveguides and links to observed dynamical processes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7081, https://doi.org/10.5194/egusphere-egu26-7081, 2026.

Building upon the established Rossby wave ray tracing framework, we introduce a phase tracing approach, derived from two-dimensional spherical Rossby wave theory on a horizontally non-uniform basic flow, to explicitly diagnose the evolution of wave crests and troughs along stationary Rossby wave rays.

The method is first applied to a series of idealized basic flows and validated against forced solutions from a barotropic model, with a particular emphasis on contrasting flows with and without a mean meridional wind. The theoretical phase tracing accurately reproduces both the ray pathways and the spatial structure of the simulated responses, in agreement with the theoretical prediction that local zonal and meridional wave scales are primarily controlled by the background flow rather than by the forcing scale. Importantly, the inclusion of a mean meridional flow emerges as a key dynamical ingredient: it not only permits one-way propagation of stationary Rossby waves across tropical easterlies, but also substantially enlarges both zonal and meridional wave scales, with the zonal scale becoming dominant, thereby shaping zonally elongated wave-train structures.

The framework is further applied to climatological summertime flows to investigate the structure of the Pacific–Japan (PJ) teleconnection. In the lower troposphere, northward-propagating Rossby waves embedded in the monsoonal southwesterly exhibit a characteristic ‘− / + / −’ phase pattern, while in the upper troposphere the phase evolution of southeastward- and southwestward-propagating Rossby waves displays a complementary ‘+ / − / +’ structure. The phase transition points along the rays are found to coincide closely with the centers of positive and negative vorticity anomalies, providing a clear dynamical explanation for the formation of the zonally elongated tripolar structure of the PJ teleconnection.

In addition, the Li–Yang wave ray flux (WRF) is employed to quantify the intensity of wave propagation along the diagnosed ray pathways, offering a complementary measure of wave activity during propagation.

Together, the phase tracing framework and wave ray flux diagnostics enable a precise and physically constrained diagnosis of atmospheric teleconnection patterns, and hold broad applicability for understanding the structure and variability of Rossby wave–mediated teleconnections in a realistic, non-uniform background flow.

How to cite: Zhao, S., Yang, Y., and Li, J.: Rossby wave phase tracing and its application to the structure of the Pacific–Japan teleconnection, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8490, https://doi.org/10.5194/egusphere-egu26-8490, 2026.

EGU26-8842 | ECS | Posters on site | AS1.20

U-Net-based Objective Detection of Atmospheric Blocking  

Hayeon Noh, Hee-Jeong Park, Jeong-Hwan Kim, Baek-Min Kim, Daehyun Kang, and Mi-Kyung Sung

Atmospheric blocking is a quasi-stationary high-pressure circulation pattern that disrupts the midlatitude westerlies and is closely linked to high-impact weather extremes. Blocking detection, however, is highly method-dependent, often producing divergent blocking climatologies. This uncertainty also affects future projections, because climate-models frequently underestimate blocking relative to observations, limiting reliable assessments of blocking-related extremes. To address these challenges, we propose an objective deep learning–based framework for blocking detection that can be applied consistently across reanalysis datasets and climate model simulations.

We frame blocking detection as identifying spatial patterns in 2D atmospheric fields, analogous to semantic image segmentation, and employ a U-Net architecture to produce daily blocking masks. A two-stage training strategy is adopted: the network is first pre-trained using labels from the standard Hybrid Index (HYB; Dunn-Sigouin et al. 2013) across all seasons and then fine-tuned with a regionally modified variant, the Regional Hybrid Index (RHYB), using boreal-winter data. This strategy allows the model to incorporate regional dependence in background variability while retraining the broad blocking characteristics learned from HYB.

Although fine-tuning is restricted to boreal winter, the trained model generalizes to boreal summer and detect additional blocking events relative to HYB. When applied to the CESM2 Large Ensemble (LESN2), the framework mitigates the tendency of traditional indices to under-detect blocking frequency. Overall, this approach offers a more objective and transferable detection method that may improve the consistency of blocking diagnostics and support more reliable evaluations of blocking-related extremes in climate-model simulations.

How to cite: Noh, H., Park, H.-J., Kim, J.-H., Kim, B.-M., Kang, D., and Sung, M.-K.: U-Net-based Objective Detection of Atmospheric Blocking , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8842, https://doi.org/10.5194/egusphere-egu26-8842, 2026.

EGU26-10101 | Orals | AS1.20

Dynamical Controls on Pacific-Origin Rossby Wave Propagation Across the North Atlantic–European Sector 

Ramon Fuentes-Franco, Julia F. Lockwood, Nick Dunstone, Adam Scaife, and Torben Koenigk

Pacific-origin atmospheric teleconnections play a central role in shaping Northern Hemisphere summer circulation, yet their downstream expression over the North Atlantic–European sector varies substantially across models. Here, we assess the robustness, structure, and background-state dependence of these teleconnections using CMIP6 large ensembles together with idealized SST-perturbation experiments from the Decadal Climate Prediction Project (DCPP-C). The study focuses on Rossby Wave Sources (RWS) over the northeastern Pacific and the resulting wavetrain that propagates across North America, the Atlantic, and Eurasia during boreal summer.

All large ensembles reproduce a coherent circumglobal Rossby wave train associated with enhanced RWS in the northeastern Pacific. However, the degree of agreement deteriorates downstream, with the largest spread occurring over the North Atlantic and Europe. Model differences in upper-tropospheric jet strength and meridional position strongly modulate the phasing and amplitude of the wave train in this region. Models with small jet biases compared to the ERA5 reanalysis maintain a realistic sequence of alternating geopotential height anomalies, while stronger or latitudinally displaced jets distort or shift the European node of the teleconnection.

Idealized DCPP-C experiments reveal that the Pacific-Atlantic interaction is strongly state-dependent. Simulations with intensified RWS (negative IPV phase) produce a PDO-like surface cooling pattern in the northeastern Pacific and a robust cooling response in the North Atlantic, confirming a direct trans-basin link. Atlantic SST anomalies further modulate the downstream atmospheric response: a warm Atlantic suppresses the Pacific–Europe teleconnection, while a cold Atlantic allows for a strengthened and more coherent wave train. Additional experiments combining AMV and IPV phases demonstrate that the Pacific signal can be either reinforced or damped depending on the Atlantic background state.

These results highlight the joint role of northeastern Pacific RWS variability, upper-level jet biases, and Atlantic SST state in shaping the structure and persistence of Pacific-to-Europe summer teleconnections. Improving the representation of these elements is essential to reduce inter-model spread and enhance confidence in simulated boreal-summer circulation patterns.

How to cite: Fuentes-Franco, R., Lockwood, J. F., Dunstone, N., Scaife, A., and Koenigk, T.: Dynamical Controls on Pacific-Origin Rossby Wave Propagation Across the North Atlantic–European Sector, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10101, https://doi.org/10.5194/egusphere-egu26-10101, 2026.

    Winter precipitation over the Tibetan Plateau (TP) and the European Alps exhibits pronounced interannual to decadal variability, yet the stability of their large-scale linkage and the associated dynamical and moisture-related processes remain incompletely understood. Using multiple observational datasets and ERA5 reanalysis for the period 1940–2018, this study examines the decadal evolution of the TP–Alps winter precipitation relationship and its connections with atmospheric circulation and moisture transport.

    The results indicate that the relationship between winter precipitation over the two regions undergoes a marked decadal transition, with contrasting behavior before and after the late twentieth century. During the earlier period, precipitation variability over the TP and the Alps displays a coherent out-of-phase structure, whereas this relationship becomes substantially weaker in subsequent decades.

    Further analyses suggest that these changes are associated with variability in large-scale climate modes linked to tropical sea surface temperature anomalies and midlatitude atmospheric circulation. Regression analyses of upper-tropospheric circulation reveal organized Rossby wave responses over Eurasia, while the corresponding wave activity flux pathways exhibit pronounced decadal dependence, indicating changes in the background circulation structure. Consistent with these circulation variations, regressions of whole-column integrated vapor transport (IVT) show notable decadal differences in the strength and pathways of moisture transport toward the TP and the Alps, with implications for regional moisture convergence.

    Overall, this study highlights the importance of large-scale circulation variability and moisture transport in shaping the decadal evolution of winter precipitation linkages over Eurasia, providing a broader context for understanding long-term hydroclimate variability across distant mountainous regions.

How to cite: Qie, J. and Wang, Y.: Decadal changes in the teleconnection of winter precipitation across Eurasian mountainous regions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11470, https://doi.org/10.5194/egusphere-egu26-11470, 2026.

EGU26-12607 | ECS | Posters on site | AS1.20

Comparison of Different Blocking Indices and Analysis of Underlying Dynamics and Synoptic Situations 

Lisa Ruff and Stephan Pfahl

Atmospheric blockings are among the most frequently studied weather patterns. They not only cause extreme weather events and associated losses but also significantly influence general weather variability. A deeper understanding and more reliable prediction of these phenomena would therefore be of great value to both the scientific community and the public.

However, various definitions and identification methods for atmospheric blockings are currently applied, which can lead to inconsistent results and confusion. While all approaches are valid and justified, the precise differences between these definitions and their implications often remain unclear.

This study examines two widely used blocking algorithms: the Anomaly Index, which is based on vertically integrated potential vorticity (PV) anomalies (see Schwierz et al., 2004), and the Absolute Index, which identifies blockings through the reversal of the 500 hPa geopotential height gradient (see Davini et al., 2012).

The two indices differ substantially already with regard to climatological blocking frequencies: the Anomaly Index primarily detects blockings south of Greenland/Iceland, whereas the Absolute Index identifies a local maximum over southern Scandinavia. Our analyses have not indicated any systematic longitudinal, latitudinal, or temporal offset between the events captured by the two indices. A synoptic investigation suggests that the algorithms detect different types of blockings: the Absolute Index requires a Rossby wave breaking for identification, while the Anomaly Index considers an extended ridge sufficient.

Further research aims to clarify the differences in dynamical and synoptic conditions between these and other algorithms.

How to cite: Ruff, L. and Pfahl, S.: Comparison of Different Blocking Indices and Analysis of Underlying Dynamics and Synoptic Situations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12607, https://doi.org/10.5194/egusphere-egu26-12607, 2026.

EGU26-14616 | Posters on site | AS1.20

Method dependence of Antarctic atmospheric blocking and implications for large-scale circulation and climate extremes 

Deniz Bozkurt, Charlie Opazo, Julio C. Marín, Kyle R. Clem, Benjamin Pohl, Victoire Buffet, Vincent Favier, Tomás Carrasco-Escaff, and Bradford S. Barrett

Atmospheric blocking is a key driver of persistent circulation anomalies and associated extreme events in the Southern Hemisphere, yet its characteristics around Antarctica remain poorly understood due to methodological diversity and the absence of a consolidated, long-term dataset. This contribution investigates how methodological choices in blocking detection influence the inferred characteristics of Antarctic blocking and discusses the implications for large-scale circulation variability and climate extremes. Using ERA5 reanalysis for the period 1979 to 2024, we apply several established blocking diagnostics based on geopotential height and potential vorticity within a unified spatiotemporal framework. By standardising filtering, event identification, tracking, and aggregation procedures, we isolate differences that arise specifically from the diagnostic formulation rather than from implementation details. The comparison reveals substantial method dependent variability in blocking frequency, spatial extent, persistence, and intensity, particularly at high southern latitudes where circulation regimes differ from classical midlatitude blocking. Geopotential height based diagnostics identify a broader range of quasi stationary anticyclonic anomalies, including events extending toward the Antarctic continent, while potential vorticity based diagnostics isolate fewer and more spatially confined events associated with dynamically coherent upper level disturbances near the polar vortex. These methodological contrasts have direct implications for how blocking related climate extremes are interpreted, including links to temperature anomalies, moisture intrusions, and surface melt episodes. Differences in diagnosed event duration and location can substantially alter the attribution of extreme conditions to blocking regimes. Ongoing work examines how blocking characteristics identified by different diagnostics relate to variability in large scale circulation modes such as the Southern Annular Mode and ENSO, highlighting the importance of methodological awareness when assessing teleconnections and long term variability. Overall, the results demonstrate that Antarctic atmospheric blocking cannot be fully characterised by a single diagnostic perspective and that method dependence must be explicitly considered in studies of polar circulation variability, climate extremes, and future change.

How to cite: Bozkurt, D., Opazo, C., Marín, J. C., Clem, K. R., Pohl, B., Buffet, V., Favier, V., Carrasco-Escaff, T., and Barrett, B. S.: Method dependence of Antarctic atmospheric blocking and implications for large-scale circulation and climate extremes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14616, https://doi.org/10.5194/egusphere-egu26-14616, 2026.

EGU26-14802 | ECS | Orals | AS1.20

A Lagrangian perspective on jet streams 

Louis Rivoire, Yohai Kaspi, Talia Tamarin-Brodsky, and Or Hadas

Synoptic systems are understood to organize heat and momentum transport along jet streams, yet the diagnostics used to identify jets remain fundamentally Eulerian in nature. This creates conceptual tension: if the eddy-driven jet can be meaningfully separated from the synoptic eddies that maintain it, then it must be a persistent flow that Eulerian diagnostics are not designed to isolate. An alternative Lagrangian perspective on jet streams (JetLag) was recently developed and identifies jets not as maxima of wind speed (or derivative variables), but as maxima of isentropic displacement. In this view, jets become persistent features that remain identifiable over synoptic timescales. This definition recovers well-known features of the atmospheric circulation, with some systematic differences relative to Eulerian diagnostics. Here we adopt the Lagrangian definition to revisit jets and their variability using a hierarchy of models, ranging from idealized configurations to reanalyses. We explore the connections between synoptic systems and jets, and those between the upper troposphere and the surface.

How to cite: Rivoire, L., Kaspi, Y., Tamarin-Brodsky, T., and Hadas, O.: A Lagrangian perspective on jet streams, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14802, https://doi.org/10.5194/egusphere-egu26-14802, 2026.

EGU26-15695 | ECS | Posters on site | AS1.20

Influences of planetary- and synoptic-scale Rossby waves on the intraseasonal variability of Yangtze River Basin precipitation in summer 

Peishan Chen, Riyu Lu, Liang Wu, Nedjeljka Žagar, and Frank Lunkeit

The Yangtze River Basin (YRB) is a critical economic and agricultural center in China, and the large summer precipitation variability here causes severe effects on social and economic. It is well known that the YRB precipitation (YRBP) is affected by multi factors, including anomalous anticyclone over the western North Pacific and local cyclone in the lower troposphere, the meridional displacement of the East Asian jet in the upper troposphere, et al. However, from the perspective of wave dynamics, influences of multi-scale Rossby waves on the intraseasonal variability of Yangtze River Basin precipitation are poorly understood. In this study, the authors used the three-dimensional multivariate circulation decomposition to quantify the multi-scale Rossby wave variability associated with the YRBP. Rossby waves with zonal wavenumber (k) being 1-20 are analyzed and categorized into planetary (k=1-3) and synoptic (k=4-20) scales, with waves of larger wavenumbers excluded due to their negligible amplitudes.  
Results indicate that the planetary- and synoptic- scale Rossby waves associated with the YRBP are favorable to the precipitation by different physical processes. On the one hand, planetary-scale Rossby waves contribute to the large-scale circulation anomalies, including the anticyclone over the western North Pacific, and the zonal cyclone over East Asia in the upper troposphere, which suggests a southward displacement of the East Asian jet. On the other hand, synoptic-scale Rosby waves are featured by a zonal wave train and contribute to local cyclonic anomalies in the lower troposphere to enhance the YRBP. 
Further lead-lag regression analysis is on-going.

How to cite: Chen, P., Lu, R., Wu, L., Žagar, N., and Lunkeit, F.: Influences of planetary- and synoptic-scale Rossby waves on the intraseasonal variability of Yangtze River Basin precipitation in summer, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15695, https://doi.org/10.5194/egusphere-egu26-15695, 2026.

Despite the ongoing global warming trend, winter temperature variability, particularly the recurrence of cold extremes across Eurasia and North America, has drawn considerable attention. These widespread anomalies suggest potentially coherent temperature variations between the two continents. Previous studies have identified the Asian–Bering–North American (ABNA) teleconnection as a key contributor to such in-phase winter temperature variations. The ABNA is characterized by a zonally elongated “negative–positive–negative” (or “positive–negative–positive”) geopotential height anomaly pattern extending across northern Asia, eastern Siberia–Alaska, and eastern North America. The ABNA is independent of, and often more dominant than, that of the ENSO-related Pacific–North American (PNA) pattern, explaining a larger portion of winter temperature variability over eastern North America. Our analysis reveals that the ABNA is intrinsically linked to the second leading mode of tropospheric thickness (a proxy for mean tropospheric temperature) variability in the Northern Hemisphere, while the first mode reflects Arctic warming. This finding positions the ABNA as a fundamental mode characterizing Eurasia–North America winter temperature co-variability. Further results show that the ABNA is modulated by both the Arctic stratospheric polar vortex (SPV) and tropical western Pacific SST anomalies. The ABNA pattern is dynamically coupled with a meridionally stretched SPV structure extending toward Eurasia and North America, forming a tropospheric bridge between the stratosphere and surface climate. This stratosphere–troposphere coupling may be initiated by Eurasian snow cover anomalies in the preceding autumn. In addition, tropical western Pacific SST anomalies can excite a poleward-propagating Rossby wave train that reinforces the ABNA pattern, in a manner comparable to but distinct from the ENSO–PNA connection. These findings highlight the ABNA as a critical and underappreciated pathway for winter climate variability and offer new sources of predictability for subseasonal-to-seasonal temperature forecasts across the Northern Hemisphere, particularly in eastern North America.

How to cite: Zhong, W. and Wu, Z.: The Asian–Bering–North American Teleconnection: A Key Mode of Winter Temperature Co-Variability Across Eurasia and North America, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15892, https://doi.org/10.5194/egusphere-egu26-15892, 2026.

The climatological quasi-stationary waves (QSW) amplitude has a distinct spatial pattern, with clear zonal asymmetries, particularly in the Northern Hemisphere; those asymmetries must be impacted by stationary forcings such as land, topography, and sea surface temperatures (SSTs). To investigate the effects of stationary forcings on QSW characteristics, including their duration and spatial distribution, we conducted eight CAM6 simulations with prescribed SSTs, spanning realistic, semi-realistic, and fully idealized configurations. Stationary forcings tend to extend the duration of QSWs and strongly impact their zonal asymmetric distribution. QSWs are primarily influenced by both the local stationary wavenumber Ks, which depends on jet speed and its second-order meridional gradient, and by the strength of transient eddies. However, the covariation between transient eddies and QSWs varies across different types of stationary forcings. For example, in experiment pairs showing the impact of zonal SST patterns, the correlation between changes in QSW strength and transient eddies is stronger, while the correlation with stationary wavenumber is of similar magnitude across all experiments. In some cases, QSW strength is also associated with the strength of the stationary waves. When the timescale of the QSWs is changed, the relative contributions from different mechanisms changes, but stationary wavenumber Ks and transient eddies strength are important in all time scales for experiments with realistic land. This work suggests that transient Rossby waves with given wavenumbers can become stationary under background conditions with the corresponding stationary wavenumbers.

How to cite: Fei, C. and White, R.: The Role of Topography, Land and Sea Surface Temperatures on Quasi-Stationary Waves in Northern Hemisphere Winter: Insights from CAM6 Simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16052, https://doi.org/10.5194/egusphere-egu26-16052, 2026.

EGU26-16164 | Posters on site | AS1.20

A role of cold air outbreak in an early winter heavy snowfall event over the Korean Peninsula 

Yujoo Oh, Eun-hyuk Baek, and Joowan Kim

Cold air outbreaks (CAOs), characterized by the southward intrusion of high-latitude cold air into the midlatitudes, often cause severe weather phenomena such as extreme cold waves and heavy snowfall during winter months. This study investigates the critical role of a CAO in a record-breaking heavy snowfall event over the Korean peninsula in November 2024. During the event, the accumulated snowfall was recorded over 43 cm across the central region of the Korean Peninsula for about 3 days, causing severe socioeconomic disasters.

Two days prior to the heavy snowfall event, an upper-level cut-off low generated over eastern Siberia propagated southward, inducing an extreme CAO over the northern Peninsula. The cut-off low enhanced an upper-level frontogenesis with tropopause folding, which transported cold and dry air downward and formed a barotropic cold dome over the region. Concurrently, the Yellow Sea located west of the Korean Peninsula exhibited anomalous high sea surface temperatures, which created an intense air-sea temperature contrast exceeding 17°C. The resulting sensible and latent heat fluxes triggered meso-scale convection, which persistently intruded into the central region of the Korean Peninsula along the southern boundary of the cold dome. It is known that CAO is often accompanied by atmospheric blocking linked to upper-level Rossby wave breaking. In this event, Kamchatka blocking prevented the upper-level cut-off low from propagating eastward and maintained it in a quasi-stationary state during about 3 days. Consequently, the unexpected CAO enhanced by quasi-stationary cut-off low and the persistent snowstorms by lake-effect resulted in the record-breaking heavy snowfall over the Korean Peninsula during early winter.

Our findings demonstrate that upper-level atmospheric circulation patterns, which have received little attention in previous studies, can play a crucial role in heavy snowfall events over the Korean Peninsula. 

 

Key words: Heavy snowfall, Cold air outbreak, cut-off low, air-sea contrast, blocking

 

This work was funded by the Korea Meteorological Administration Research and Development Program under Grant (RS-2023-00240346)

How to cite: Oh, Y., Baek, E., and Kim, J.: A role of cold air outbreak in an early winter heavy snowfall event over the Korean Peninsula, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16164, https://doi.org/10.5194/egusphere-egu26-16164, 2026.

EGU26-16728 | ECS | Orals | AS1.20

A simple statistical approach for establishing dynamical linkages between specific atmospheric circulation patterns and spatially compounding persistent extremes and impacts 

Dominik Diedrich, Miguel Lima, Ricardo Trigo, Ana Russo, Giorgia Di Capua, Guruprem Bishnoi, and Reik V. Donner

During the last years, the statistical analysis of compound extremes has gained increasing interest among the scientific community due to the multiple threats posed by such events to society, economy, and the environment. In many situations, this analysis is based on bivariate extreme value theory and measures provided by this framework. Such methods may however not properly address two relevant aspects: the non-zero duration of extreme events (which can be rather persistent, e.g. in the case of droughts or heatwaves, heavily violating the independence assumption of classical extreme value theory) and the fact that not all events of practical relevance can actually be described as cases falling into the tails of the continuous distribution of some observable of interest.

A versatile approach addressing the non-extremeness aspect is event coincidence analysis (ECA), which quantifies the empirical frequency of co-occurring events of arbitrary types and allows its comparison with the values for certain random null models like independent Poisson processes with prescribed event rates. While standard ECA builds upon the concept of temporal point processes and hence may be criticized for not applying to persistent events, a new methodological variant called interval coverage analysis (InCA) provides a straightforward generalization specifically addressing co-occurrence properties of persistent events. To highlight the broad range of potential applications of ECA and InCA in the context of compound event studies, we study two examples of co-occurrences between specific atmospheric circulation configurations and different types of surface extremes.

Example 1 highlights the instantaneous as well as time-lagged co-occurrence between boreal summer Northern hemispheric jet stream configurations with two distinct zonal wind maxima (“double jet”) and atmospheric heat waves. The presented results demonstrate that double jet conditions over certain sectors are closely linked with a statistically significant enhancement or suppression of heatwave activity in distinct regions, resembling the spatial patterns of atmospheric wave trains. These patterns provide a useful starting point for further targeted research to reveal the underlying atmospheric circulation mechanisms and their association with other spatially compounding extreme events and impacts.

Example 2 subsequently addresses the co-occurrence of subtropical ridges and atmospheric blockings with precipitation patterns in the Southern hemisphere. The obtained results indicate that the presence of ridges in specific sectors is commonly accompanied by a suppression of precipitation within these sectors, while surrounding regions may exhibit characteristic spatial clusters of significantly elevated probability of precipitation.

This work has been partially supported via the JPI Climate/JPI Oceans NextG-Climate Science project ROADMAP and the bilateral German-Portuguese science exchange project EXCECIF (jointly funded by DAAD and FCT).

How to cite: Diedrich, D., Lima, M., Trigo, R., Russo, A., Di Capua, G., Bishnoi, G., and Donner, R. V.: A simple statistical approach for establishing dynamical linkages between specific atmospheric circulation patterns and spatially compounding persistent extremes and impacts, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16728, https://doi.org/10.5194/egusphere-egu26-16728, 2026.

EGU26-19201 | Orals | AS1.20

Perturbation and uncertainty growth along the jet stream: the role of tropical cyclones, jet stream dynamics, and sensitivity to resolution 

Mark Rodwell, Aristofanis Tsiringakis, Suzanne Gray, John Methven, and Doug Wood

We investigate the development of ensemble forecast uncertianty associated with jet stream perturbations and dynamics. We partition uncertainty growth into diabatic and dynamic processes. A case study focusses on the recent Fujiwara-style interaction of Hurricanes Humberto and Imelda , and their subsequent interactions with the jet stream. These are seen to be able to perturb the jet and inject considerable uncertainty via diabatic processes. Later, dynamical processes along the jet (such as the development of cut-of features) act to further magnify uncertainty. The result for Europe was Storm Amy, which caused significant damage and some loss of life, but which was not well predicted. Through further experimentation, we try to understand the key diabatic and dynamical processes, how they combine to govern operational predictive skill, and their sensitivity to model resolution.

How to cite: Rodwell, M., Tsiringakis, A., Gray, S., Methven, J., and Wood, D.: Perturbation and uncertainty growth along the jet stream: the role of tropical cyclones, jet stream dynamics, and sensitivity to resolution, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19201, https://doi.org/10.5194/egusphere-egu26-19201, 2026.

EGU26-19251 | Orals | AS1.20

Do Rossby wave packet envelopes exhibit enhanced predictability? 

Michael Riemer and Lorenz Gölz

Rossby wave packets (RWPs) organize large-scale energy transport in the atmosphere. The significance of this energy transport for atmospheric predictability and teleconnections has long been recognized. We here focus on RWPs along the midlatitude jet, which have received much attention as predictable precursors to high-impact weather events. RWPs are frequently considered as physical entities identified by the Rossby-wave envelope. From this perspective, RWPs appear as features on a scale larger than that of the underlying troughs and ridges. In particular, a long-standing hypothesis by Lee and Held (1993) states that "the packet envelope should be more predictable than the individual weather systems, because the packet can remain coherent despite chaotic internal dynamics". Testing this hypothesis with ERA5 re-forecasts, we find that the RWP envelope does not exhibit this hypothesized higher predictability, at least when compared to the pattern of the underlying Rossby waves themselves, and until the end of the available lead time range of 10 days. This statistical result is substantiated by the examination of the underlying error-growth mechanisms. We will further provide a dynamics-based explanation of the counterintuitive result that the (seemingly) larger-scale envelope feature does not exhibit higher predictability. We conclude the presentation with a discussion of the role of the envelope perspective for predictability questions beyond the medium range.

How to cite: Riemer, M. and Gölz, L.: Do Rossby wave packet envelopes exhibit enhanced predictability?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19251, https://doi.org/10.5194/egusphere-egu26-19251, 2026.

EGU26-19340 | Orals | AS1.20

Concurrent heat waves and their linkage to large-scale meridional heat transports through planetary-scale waves 

Valerio Lembo, Gabriele Messori, Davide Faranda, Vera Melinda Galfi, Rune Grand Graversen, and Flavio Emanuele Pons

There is increasing interest within the community in the mechanisms behind the development of concurrent heatwaves, i.e., heatwaves that occur simultaneously in geographically remote regions. This interest is motivated by their socio-economic implications and by the fact that they are occurring more frequently with global warming.

While the large-scale atmospheric dynamical drivers of concurrent heatwaves have often been emphasized, with a focus on quasi-stationary wave patterns favoring the formation of blockings, particularly in Summer, the thermodynamic drivers have so far received less attention, despite the recognized role of moisture and latent heat transport for the development of blockings, especially in Winter.

Here, we relate extremes in hemispheric meridional heat transport (MHT) to occurrences of hemispheric land-surface temperature (LST) warm and cold extremes. We find that the combination of extremely weak MHT and extremely warm hemispheric LST days occurs significantly more often than other combinations, and that these events are associated with a substantial amount of concurrent heatwaves in the Northern Hemisphere mid-latitudes, both in boreal Winter and Summer. We highlight that, in Summer, the phase and amplitude of high-latitude blockings associated with these occurrences lead to vanishing, and sometimes even equatorward, overall MHT, together with an intensification of the Pacific branch of the jet stream. In Winter, MHT is largely suppressed by an excessively zonal flow, bringing mild and moist air towards continental regions, both in Eurasia and North America. The reversal or suppression of zonal wavenumber-2 and -3 contributions to MHT is found to be related to these MHT extremes, pointing towards the predominant role of ultra-long planetary-scale waves.

How to cite: Lembo, V., Messori, G., Faranda, D., Galfi, V. M., Graversen, R. G., and Pons, F. E.: Concurrent heat waves and their linkage to large-scale meridional heat transports through planetary-scale waves, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19340, https://doi.org/10.5194/egusphere-egu26-19340, 2026.

EGU26-19586 | Posters on site | AS1.20

Jet regimes, waviness metrics, and links to extreme weather 

Ruth Geen, Myles Jones, Ruby Riggs, and Yuran Cao

Extreme midlatitude weather is often associated with pronounced Rossby waves. This has motivated interest in how the ‘waviness’ of the atmosphere is changing as Earth warms. Multiple summary metrics have been used to assess midlatitude waviness, which include both descriptions of the magnitudes of associated anomalies in geopotential height, and geometric measures of deviations of the jet from a more zonal state.

Recent work illustrated that a) these metrics can respond differently to warming, and that the same metric can respond differently to warming applied in different ways (Geen et al. 2023), and b) that different metrics can link to rather different patterns of extreme temperature (Roocroft et al. 2025). It remains unclear what specific types of characteristic jet structures these various metrics capture, and how these dynamically link to surface weather extremes.

Here, we first explore how different metrics relate to extreme winter weather events (cold, rain and wind) over Europe and North America, and how these relationships compare to known modes of climate variability such as the NAO. Next, to explore underlying jet structures driving these extremes, we apply a Self Organising Maps analysis to 500-hPa geopotential height anomalies. This allows us to map the values taken by different metrics and the likelihoods of extreme events for different jet configurations in a reduced dimensionality space.

 

References

Geen, R., Thomson, S. I., Screen, J. A., Blackport, R., Lewis, N. T., Mudhar, R., ... & Vallis, G. K. (2023). An explanation for the metric dependence of the midlatitude jet‐waviness change in response to polar warming. Geophysical Research Letters, 50(21), e2023GL105132.

Roocroft, E., White, R. H., & Radić, V. (2025). Linking atmospheric waviness to extreme temperatures across the Northern Hemisphere: Comparison of different waviness metrics. Journal of Geophysical Research: Atmospheres130(20), e2024JD042631.

How to cite: Geen, R., Jones, M., Riggs, R., and Cao, Y.: Jet regimes, waviness metrics, and links to extreme weather, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19586, https://doi.org/10.5194/egusphere-egu26-19586, 2026.

EGU26-20078 | ECS | Posters on site | AS1.20

Dynamical linkage between blocking predictability and jet stream quasi-stationary states 

Suzune Nomura and Takeshi Enomoto

This study investigates atmospheric blocking from the perspective of the instantaneous stationarity of the jet stream. The framework of the quasi-stationary state (QS) dynamical theory is applied to characterize the behavior of ensemble prediction members. Using the Japanese Reanalysis for Three Quarters of a Century (JRA-3Q), we classified atmospheric conditions over the Northern Hemisphere into states characterized by small and large temporal variability in jet stream tendency, referred to as QS and Non-QS respectively, and examined the relationship between the former and blocking patterns.

During QS conditions, the westerlies exhibited significant meandering, and blocking occurred regardless of the blocking type (Omega or Dipole). These results are consistent with blocking defined by potential vorticity reversal at the dynamical tropopause and its persistence.

Based on linearized equations, a relationship is identified between QS and the non-stationary minimum point (MP), where at least one of its eigenvalues is zero. Analysis of forecast data from JMA's Global Ensemble Prediction System (GEPS) revealed that ensemble spread tends to increase with forecast time when the initial state is QS. This result is consistent with the proposed dynamics. Conversely, under a Non-QS initial state, initial uncertainty persists throughout forecast evolution.

These findings suggest that atmospheric blocking is a manifestation of the instantaneous stationarity of the jet stream, indicating that this theoretical framework is valuable for examining the predictability of blocking and interpreting ensemble forecasts.

How to cite: Nomura, S. and Enomoto, T.: Dynamical linkage between blocking predictability and jet stream quasi-stationary states, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20078, https://doi.org/10.5194/egusphere-egu26-20078, 2026.

EGU26-20138 | ECS | Orals | AS1.20

Linking jet stream and Rossby wave spectra changes within internal variability and climate change responses 

Zhenghe Xuan, Jacopo Riboldi, and Robert Jnglin Wills

The occurrence and magnitude of extreme events have been linked to quasi-stationary waves (QSW). However, the response of QSWs to climate change is uncertain. Here, we gain insight into the forced QSW response by looking at internal variability in QSW activity. The Rossby wave spectra is highly influenced by the location and strength of the background jet stream. It is known that the poleward shift of the jets in response to external forcing resembles internal variability in the jet such as the Southern Annular Mode. Although open questions remain on the driving mechanisms of these jet responses, we can identify common changes in the Rossby wave spectra within internal variability and the climate change response. 

Using the daily meridional velocity from the Community Earth System Model 2 Large Ensemble, we calculate a space-time spectral decomposition over the midlatitudes, revealing changes in the wavenumber-phase speed structure of synoptic Rossby waves. We investigate the climate change response of the spectra and use maximum covariance analysis between the spectra and the vertically integrated zonal wind to find co-varying patterns of internal variability. Under the SSP3-7.0 scenario in the Southern Hemisphere, we observe a polewards shift of the jet, faster jet speeds, and a corresponding shift of the spectra perpendicular to the barotropic Rossby wave dispersion relationship. This results in a decrease in power in higher wavenumbers and an increase in lower wavenumbers across all phase speeds, including quasi-stationary ones, corresponding to a decrease in stationarity (i.e. wave power with near-zero phase speed). We find this relationship holds on monthly timescales and in response to climate change. The response in the Northern Hemisphere is more complex and differs between the Atlantic and Pacific basin. Our results provide a simple explanation for the wavenumber-dependent changes in Rossby waves and the reduced stationarity of QSWs in response to climate change, which have implications for future changes in weather extremes.

How to cite: Xuan, Z., Riboldi, J., and Jnglin Wills, R.: Linking jet stream and Rossby wave spectra changes within internal variability and climate change responses, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20138, https://doi.org/10.5194/egusphere-egu26-20138, 2026.

EGU26-20715 | ECS | Orals | AS1.20

European Heatwave Exacerbated by Summer Arctic Changes 

El Noh, Joowan Kim, Yu Kosaka, Sang-Wook Yeh, Seok-Woo Son, Sang-Yoon Jun, and Woosok Moon

Since 2010, European heatwaves have dramatically escalated in both duration and severity. The cumulative intensity of European heatwaves has surged by over 50% in the recent decade. Recent studies have reported accelerating Arctic warming and associated mid-latitude circulation changes. However, its summer impacts remain uncertain. Here we provide evidence that the recent summer changes in the Arctic play a critical role in the escalation of European heatwaves. The Arctic has experienced unprecedented regional changes with substantial sea-ice loss since 2010. The Barents-Kara Seas have warmed by 2.3 °C per decade, while western Greenland has cooled by 0.6 °C per decade. The temperature changes in these two regions influenced European weather through two different pathways: 1) Barents-Kara Sea warming weakened daily weather activities over western Eurasia, thereby promoting persistently hot weather; 2) Greenland cooling shifted the North Atlantic jet stream, which allowed easy invasion of warm flows from the subtropics and Sahara. These pathways have intensified concurrently since 2010, which likely exacerbates heatwave risks in Europe. 

How to cite: Noh, E., Kim, J., Kosaka, Y., Yeh, S.-W., Son, S.-W., Jun, S.-Y., and Moon, W.: European Heatwave Exacerbated by Summer Arctic Changes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20715, https://doi.org/10.5194/egusphere-egu26-20715, 2026.

The response of upper-tropospheric jet streams to warming effects is a pivotal uncertainty in current climate projections. This study provides a rigorous diagnostic analysis of the spatio-temporal variability and seasonal evolution of jet stream characteristics over North America (NA) and the North Pacific Ocean (NPO) during the four-decade period of 1984-2023. Utilizing high-resolution ERA5 and NCEP/NCAR reanalysis datasets, we analyzed the three-dimensional structure of jet cores and their interaction with localized baroclinic environments.

Our diagnostics reveal two distinct centers of action where jet dynamics are significantly perturbed: the North Pacific Ocean (NPO) and the Eastern portion of North America (EPNA). A systematic poleward migration of the jet axes approximately 10 degrees in latitude is identified across all seasons except summer, concurrent with a persistent altitudinal ascent. Seasonal analysis indicates that trajectory instability reaches its maximum during summer in the NPO, whereas the most pronounced variability in EPNA occurs during the autumn months. Notably, our results establish a significant positive trend in zonal wind speeds, ranging from 0.5 to 1.5 m/s per decade, which is closely coupled with enhanced meridional temperature gradients in the mid-to-upper troposphere.

Furthermore, wavelet power spectrum analysis across multiple pressure levels (100-400 hPa) uncovers dominant multi-annual periodicities of 5, 7, and 10 years, suggesting robust modulation by large-scale climatic oscillations. A critical finding is the divergent altitudinal behavior between the two regions: while NPO jet streams exhibit an upward trend with stabilized flow, winter and autumn jet streams over EPNA demonstrate a significant downward intrusion into the lower troposphere. This vertical shift facilitates intensified moisture advection from the Gulf of Mexico, potentially exacerbating the frequency and magnitude of extreme hydrological events, such as atmospheric rivers, in northeastern Canada. These findings underscore the non-uniform regional response of the global circulation to a warming atmosphere and provide a framework for improving regional climate predictability.

How to cite: Salimi, S. and Ouarda, T. B. M. J.: Decadal Evolution of Mid-latitude Jet Stream Dynamics: Spatio-temporal Trends and Seasonal Oscillations over North America and the North Pacific Ocean, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21982, https://doi.org/10.5194/egusphere-egu26-21982, 2026.

EGU26-23268 | Posters on site | AS1.20

Atmospheric waveguides, quasi-stationary waves, and temperature extremes 

Rachel White and Lualawi Mareshet Admasu

Atmospheric waveguides can affect the propagation of Rossby waves, and have been hypothesized to be associated with amplified quasi-stationary waves and thus to extreme weather events in the mid-latitudes. Here, we compare different methods of calculating temporally and spatially varying waveguides, including different ways of separating the waveguides (background flow) from waves, and show that upstream PV waveguides are often present in the days prior to heatwaves. We compare waveguides from potential vorticity (PV) gradients (“PV waveguides”) with barotropic waveguides based on what is known as the stationary wavenumber, or KS (“KS waveguides”). Composites of days with high waveguide strength over particular regions show distinct differences between the two waveguide definitions. Strong KS waveguides in many regions are associated with a double-jet structure, consistent with previous research; this structure is rarely present for strong PV waveguides. The presence of high geopotential heights occurs with the double-jet anomaly, consistent with atmospheric blocking creating the KS waveguide conditions through the influence on local zonal winds, highlighting that this methodology does not sufficiently separate non-linear perturbations (i.e. blocking) from the waveguides, or background flow. Significant positive correlations exist between local waveguide strength and the amplitude of quasi-stationary waves; these correlations are stronger and more widespread for PV waveguides than for KS waveguides, and they are strongest when the rolling-zonalization background flow method is used. We caution against using KS waveguides on temporally and/or zonally varying scales and recommend rolling-zonalization PV waveguides for the study of waveguides and their connections to quasi-stationary atmospheric waves. Using PV waveguides, we find strong connections with heatwaves, with enhanced waveguides upstream from 1-6 days prior to heatwave days.

How to cite: White, R. and Admasu, L. M.: Atmospheric waveguides, quasi-stationary waves, and temperature extremes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-23268, https://doi.org/10.5194/egusphere-egu26-23268, 2026.

EGU26-247 | Posters on site | HS3.4

Addition of Process-Based Stream Temperature Modeling Capabilities to MODFLOW 6 

Eric Morway, Katie Fogg, Alden Provost, Christian Langevin, Joseph Hughes, and Martijn Russcher

MODFLOW is a well-known and widely used groundwater flow simulator.  Characteristics that have historically defined MODFLOW remain in place: it is open-source, freely available, well-documented, and intuitive.  A complete rewrite of MODFLOW in 2017 has facilitated the adoption of several new model types embedded directly into the MODFLOW framework.  In addition to simulating groundwater flow, MODFLOW 6 now also includes solute transport, particle tracking, and a new heat-transport model called the Groundwater Energy (GWE) transport model.  Many other enhancements are actively being developed.  As with all model types available within the MODFLOW 6 hydrologic simulator, the GWE model leverages the design concept commonly referred to as packages – modules that represent specific features of the hydrologic system being modeled.  For example, the Streamflow Routing (SFR) package can be activated to simulate flow in streams.  If desired, users also can simulate heat transport within a stream network by activating the Streamflow Energy (SFE) transport package.  The SFE package simulates advective heat transport within the stream network while also accounting for advective and conductive heat exchange with the underlying groundwater system.  Although the initial release of GWE offered basic heat transport functionality in stream networks through the SFE package, detailed representation of heat exchange between stream reaches and the atmosphere was not included.  However, recent SFE development efforts are focused on adding functionality to represent heat exchange with the atmosphere.  New processes by which heat may be exchanged with the atmosphere are short- and long-wave radiation and sensible and latent heat fluxes.  When finished, the new process-based stream temperature modeling capabilities will work with the other MODFLOW features, including the application programming interface (API), parallel simulation, the input data model (IDM), and support within the popular FloPy Python library.

How to cite: Morway, E., Fogg, K., Provost, A., Langevin, C., Hughes, J., and Russcher, M.: Addition of Process-Based Stream Temperature Modeling Capabilities to MODFLOW 6, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-247, https://doi.org/10.5194/egusphere-egu26-247, 2026.

EGU26-1167 | ECS | Posters on site | HS3.4

Enhancing Streamflow Simulations Through Input Data Denoising 

Injila Hamid and Vinayakam Jothiprakash

Hydrological models are vital for understanding water resources and their responses to environmental and climatic changes, but their accuracy depends strongly on input data quality. This study evaluates how noise reduction in meteorological inputs influences the performance of the SWAT hydrological model for the lower Columbia River basin. Wavelet Transform (WT) was applied for partial denoising, while Singular Spectrum Analysis (SSA) was used for both partial and full noise removal. SSA allows extraction of trend, periodic, and noise components individually from time series data. Results indicate that partial denoising using WT significantly improves model performance, increasing the correlation coefficient (r) and Nash–Sutcliffe Efficiency (NSE) by 2 to 5%, Kling-Gupta Efficiency (KGE) by 16%, and reducing RSR by 4%, along with a notable reduction in PBIAS (from −4.7 to +1.3). The partially denoised WT model achieved r = 0.91, NSE = 0.81, PBIAS = 1.30, KGE = 0.88, and RSR = 0.45, outperforming both the base and fully denoised models. The comparative analysis shows that completely removing noise offers limited benefits and may suppress natural variability, while partial denoising provides an optimal balance between data reliability and model precision. These findings highlight the importance of appropriate input-data preprocessing in improving hydrological model performance and reducing uncertainty in water resource assessments.

How to cite: Hamid, I. and Jothiprakash, V.: Enhancing Streamflow Simulations Through Input Data Denoising, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1167, https://doi.org/10.5194/egusphere-egu26-1167, 2026.

EGU26-1351 | ECS | Orals | HS3.4

Geostatistical active learning for expanding monitoring networks for environmental decision making 

Felix Henkel, Jonathan Frank, Thomas Suesse, and Alexander Brenning

The expansion and optimisation of environmental monitoring networks requires the efficient use of limited resources to improve spatial predictions to ensure the protection of human health and ecosystems.

Network densification is a spatial sampling problem that is often addressed by pointwise-prediction uncertainty approaches, which ignore (1) the impact of a new site on its neighbourhood and (2) the binary decision task motivating the monitoring. Active learning (AL) is a machine learning technique that iteratively selects new locations based on the current maximum uncertainty in the available training data. We therefore recast network densification as an AL task and propose model-agnostic acquisition criteria, including a decision-aligned focal logit criterion that prioritises neighbourhoods whose exceedance probabilities lie near regulatory thresholds. A look-ahead criterion based on the expected reduction in prediction standard error (SE) is also examined. In a groundwater nitrate concentration case study, the focal logit criterion consistently selected more informative sites than traditional dispersion- or prediction-SE-based criteria, yielding up to 58 % greater gains in exceedance-mapping accuracy (Cohen’s κ)). Focal logit and SE criteria outperformed pointwise counterparts by ~45 % on average, while the look-ahead criterion performed well but at much higher computational cost.

The proposed framework is simple, generalisable to other environmental pollutants (such as air pollutants), and supports a transparent, decision-oriented monitoring design.

How to cite: Henkel, F., Frank, J., Suesse, T., and Brenning, A.: Geostatistical active learning for expanding monitoring networks for environmental decision making, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1351, https://doi.org/10.5194/egusphere-egu26-1351, 2026.

Decisions concerning the management of natural resources are often based on binary criteria that determine whether a specific environmental target is met or exceeded. A common example is the designation of “polluted” areas, where mitigation measures must be implemented once concentrations surpass a regulatory threshold. In practice, maps of such exceedances are commonly derived from regionalized concentration estimates. However, most conventional spatial interpolation and prediction procedures introduce systematic bias in the estimated extent of polluted areas.

To overcome this issue, we apply a bias-corrected mapping procedure that is compatible with any geostatistical or machine learning method capable of providing valid probability estimates. For the case study, we mainly focus on a trans-Gaussian regression-kriging (TRGK) framework, selected for its interpretability and transparent decomposition of predictions. To assess the potential added value of nonparametric approaches, we additionally compare TRGK with quantile regression forest (QRF) in a sub-region.

The TRGK model follows a structured, non-stationary design: (i) raw concentrations are transformed to log10 scale; (ii) a nationwide global linear model captures broad-scale relationships; (iii) major hydrogeological districts serve as units for local linear refinements to account for non-stationarity; (iv) residuals are transformed using a Gaussian anamorphosis; and (v) the transformed residuals are interpolated via ordinary kriging, from which probability estimates are derived. This setup improves flexibility while maintaining interpretability and coherent uncertainty quantification.

Bias correction is performed by estimating the total exceedance area implied by the data and determining a calibrated probability threshold that ensures an unbiased delineation of the polluted area. In this study, we jointly evaluate a threshold exceedance criterion and a temporal trend criterion.

Groundwater nitrate mapping at national scale represents a challenging test case due to strong non-normality, spatial heterogeneity, and pronounced non-stationarity. The approach nonetheless performs robustly. Linear model components exhibit R2 values between 0.15 and 0.62, while semivariogram practical ranges vary from 0.3 to 22.3 km. In the sub-region comparison, QRF showed a small discrimination advantage over TRGK (AUC 0.86 vs. 0.82) but relied more heavily on calibration (underestimation without calibration 94.9% vs. 5.1%).

Overall, the results demonstrate that the bias-corrected probability-based framework provides a flexible, robust and- when coupled with geostatistics- transparent solution for large-scale pollution mapping.

How to cite: Frank, J., Suesse, T., Jiang, S., and Brenning, A.: Bias-corrected pollution mapping with non-stationary geostatistics and spatial machine learning for environmental decision making: The case of groundwater nitrate, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1406, https://doi.org/10.5194/egusphere-egu26-1406, 2026.

Hydrological extreme records in many regions in the world may include observations from different genesis and levels of extremeness forming a characteristic “separation phenomenon’ that limits the effectiveness of traditional distributions such as the Gumbel and log-Pearson Type III models, and in such mixed extreme populations, the Two-Component Extreme Value (TCEV) distribution is better suited. However, conventional fitting approaches tend to emphasize the abundant ordinary data because of the scarcity of right-tail observations, which results in inaccurate predictions of high quantiles. Nevertheless, accurate representation of the upper tail (i.e., the high-value ranges of the cumulative distribution function, CDF) is essential for flood risk evaluation and the design of hydraulic structures. To address this issue, this study introduces a new TCEV fitting approach (SR-MWS) aimed at improving right-tail performance. In the new proposal, the dataset is first approximated using a piecewise two linear regression, and the slope ratio between the two parts (R = S1/S2) is used to assess whether TCEV modeling is appropriate or not (if R > 1.5, the dataset is regarded as suitable for TCEV fitting). Following, three weighting strategies—linear, quadratic, and exponential—are applied sequentially to obtain the final TCEV parameters. A partitioned scoring framework is then used to select the most suitable weighting scheme, emphasizing the mid-to-upper CDF range F(x) ∈ [0.6, 1.0], which corresponds to return periods from about 2.5 years to more than 200 years, while also considering overall fit quality. Our results show that the proposed method yields more accurate estimates for extreme values than conventional techniques and exhibits consistent performance for both peak-flow and precipitation datasets. Beyond hydrological applications, it provides an automated and robust tool for modeling extreme events and supporting risk assessment in fields characterized by mixed-population data with a pronounced dog-leg structure.

How to cite: Valdes-Abellan, J., Ta, L., and Yu, C.: New Proposal for maximum hydrological events fitting showing the ‘separation phenomenon’ with flexible TCEV Distribution , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1449, https://doi.org/10.5194/egusphere-egu26-1449, 2026.

EGU26-1813 | Orals | HS3.4

Residual error modelling for hourly streamflow predictions 

Cristina Prieto, Dmitri Kavetski, Fabrizio Fenicia, James Kirchner, David McInerney, Mark Thyer, and César Álvarez

 Statistical residual error modelling for hourly streamflow predictions

Cristina Prieto1,2,3, Dmitri Kavetski4,1, Fabrizio Fenicia3, James Kirchner2,5,6, David McInerney4, Mark Thyer4, and César Álvarez1

 

(1) IHCantabria—Instituto de Hidráulica Ambiental de la Universidad de Cantabria, Santander, Spain

(2) Department of Environmental Systems Science, ETH Zürich, Zürich, Switzerland

(3) Eawag, Swiss Federal Institute of Aquatic Science and Technology, Dübendorf, Switzerland

(4) School of Civil, Environmental and Mining Engineering, University of Adelaide, Adelaide, SA, Australia

(5) Swiss Federal Research Institute WSL, Birmensdorf, Switzerland

(6) Department of Earth and Planetary Science, University of California, Berkeley, California, USA

 

Water plays a critical role in societal stability through both its excess and scarcity. Extreme hydrological events can cause substantial human and economic losses, while water scarcity affects essential services such as drinking water supply, food production, and hydropower generation. Reliable streamflow predictions are therefore fundamental for environmental assessments, flood risk management, and Integrated Water Resources Management (IWRM).

Hydrological models are central tools for understanding catchment behaviour and generating predictions to support water-resources assessment, planning, and management. However, their predictive performance strongly depends on the temporal resolution at which they are applied.

At hourly time scales, hydrological processes and associated uncertainties become markedly more complex, particularly in small and mesoscale catchments. Flood peaks may last only a few hours, so daily streamflow predictions can substantially underestimate peak magnitudes; antecedent wetness conditions can evolve rapidly; and the dominant processes controlling short-term streamflow dynamics differ from those governing longer term behavior. For example, over longer time scales, predictions are primarily constrained by mass balance, whereas short-term predictions depend more strongly on dynamics and flow routing.

In addition to classical sources of uncertainty related to data, model structure, and parameters, hourly streamflow predictions often exhibit bias, heteroscedasticity, temporal autocorrelation, and non-stationarity.

Despite their importance, hourly streamflow prediction and uncertainty characterisation have received comparatively less attention than daily-scale studies.

In this work, we use a conceptual hydrological model to generate deterministic hourly streamflow predictions and quantify predictive uncertainty using a residual error modelling framework. Case-study catchments include hydrologically diverse basins in Europe and the United States. Bias, heteroscedasticity, and temporal dependence in model residuals are addressed using Box–Cox transformations and autoregressive and moving average (ARMA) models.

Results indicate that a logarithmic transformation combined with an autoregressive model of order three (AR(3)) provides the most consistent performance across catchments. This work advances streamflow prediction by developing statistically rigorous methods for post-processing the residuals of conceptual hydrological models at the hourly time scale, supporting more reliable hourly streamflow predictions for integrated water resources management and decision-making.

How to cite: Prieto, C., Kavetski, D., Fenicia, F., Kirchner, J., McInerney, D., Thyer, M., and Álvarez, C.: Residual error modelling for hourly streamflow predictions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1813, https://doi.org/10.5194/egusphere-egu26-1813, 2026.

EGU26-3193 | ECS | Orals | HS3.4

Designing Sampling Strategies for the Efficient Estimation of Parameterized Spatial Covariance Models 

Olivia L. Walbert, Frederik J. Simons, Arthur P. Guillaumin, and Sofia C. Olhede

Spatial data in the Earth and environmental sciences acquired by instrument collection or simulation are constrained to finite, discrete, (ir)regular grids whose geometry is delineated by a boundary within which missingness, either random or structured, may exist. We model (ir)regularly sampled Cartesian spatial data as realizations of discrete two- and three-dimensional random fields whose covariance structure we estimate parametrically with a spectral-domain maximum-likelihood estimation strategy using the debiased Whittle likelihood, which efficiently counters the effects of aliasing and spectral leakage that arise from finite sampling and boundary effects. We work with the general, flexible Matérn class of covariance functions, which characterizes the shape of a field through three parameters that quantify its amplitude, smoothness, and correlation length. We quantify parameter covariance analytically and asymptotically based on the parametric model and sampling grid alone, agnostic of observed data. Our uncertainty quantification allows us to study how sampling geometry imparts uncertainty on a covariance model and provides a path for optimizing the design of a sampling grid to reduce error for an anticipated model. We formulate several approaches for interrogating our model residuals to interpret where real Earth data depart from the null hypotheses of Gaussianity, stationarity, and isotropy. We explore select case studies that demonstrate the broad applicability of our models across Earth science disciplines and develop software in MATLAB and Python for implementation by domain scientists, in hydrology, and elsewhere.

How to cite: Walbert, O. L., Simons, F. J., Guillaumin, A. P., and Olhede, S. C.: Designing Sampling Strategies for the Efficient Estimation of Parameterized Spatial Covariance Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3193, https://doi.org/10.5194/egusphere-egu26-3193, 2026.

Spatial and temporal datasets that comprise distributions of events along a transect/timeline together with their magnitudes can display scale-dependent changes in persistence or anti-persistence that may contain signatures of underlying physical processes. Lacunarity is a technique that was originally developed for multiscale analysis of data and characterizes the distribution of spaces or gaps in a pattern as a function of scale. In this study, we demonstrate how lacunarity may be modified in order to reveal scale-dependent changes in 1-dimensional data related to fractures, sedimentary layering and rainfall. In order to address whether fractures found along a 1-dimensional transect (scanline) occur in clusters, we compare the lacunarity of a given fracture-spacing data to a theoretical random lacunarity curve. Further, we introduce the concept of 1st derivative of log-transformed lacunarity and demonstrate that this function can find the inter-cluster spacing and possible fractal behaviour over certain scales. It will be demonstrated how this same technique may be applied to a time-series, e.g., rainfall data, to see whether such events occur in clusters over certain time-scales. Next, the “event magnitudes” (e.g., fracture aperture) were added to each event data point (e.g., fracture) thus, yielding a 1-dimensional non-binary dataset and it was tested whether the dataset shows scale-dependent changes in terms of anti-persistence and persistence. The concept of lacunarity ratio, LR, is introduced, which is the lacunarity of a given dataset normalized to the lacunarity of its random counterpart. This randomization however, is different from the one used in the previous technique. In case of our fracture dataset for example, the random sequence is generated by leaving the locations of fractures unaltered and randomly reallocating the magnitudes along the dataset. It was demonstrated that LR can successfully delineate scale-dependent changes in terms of anti-persistence and persistence. In addition to the fracture data already mentioned here (spacing and apertures from NE Mexico), the one used for developing this technique, it was applied to two different types of data: a set of varved sediments from Marca Shale and, a hundred-year rainfall record from Knoxville, TN, USA. While the fracture data showed anti-persistence at small scales (within cluster) and random behavior at large scales, the rainfall data and varved sediments both appear to be persistent at small scales becoming random at larger scales. It was no surprise to find such striking similarity between the spatial “sedimentary” data and the time-dependent rainfall data because in rock records, the former is often considered to be a proxy for the latter. In general, such differences in behavior with respect to scale-dependent changes in anti-persistence to random, persistence to random, or otherwise, maybe be related to differences in the physicochemical properties and processes contributing to multiscale datasets.

How to cite: Roy, A. and Mukerji, T.: Identifying Scale-dependent Spatial and Temporal Patterns in Earth Science Data: Lacunarity-based Techniques, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4505, https://doi.org/10.5194/egusphere-egu26-4505, 2026.

EGU26-5236 | Orals | HS3.4

Which grid points are statistically significant? Revisiting false discovery rate correction in geospatial data 

Michael Schutte, Leonardo Olivetti, and Gabriele Messori

Scientific publications in the geosciences routinely assess statistical significance in spatially distributed environmental and geophysical data. When statistical significance is indicated, it is most often assessed independently at each grid point, while formal adjustment for multiple testing is rarely applied. However, applying multiple testing corrections, such as the global false discovery rate (FDR) approach is not always straightforward, as environmental and geophysical data are often spatially correlated.

In our work, we highlight how neglecting multiple testing correction can substantially inflate the number of false positives. We further show that commonly used FDR implementations can yield counterintuitive and potentially misleading results when applied to strongly spatially correlated data.

To illustrate the latter point, we provide an example based on near-surface air temperature composites following sudden stratospheric warmings. We first show that when anomalies are spatially coherent, restricting the spatial domain can increase the FDR-adjusted significance threshold. As a result, the same underlying field may display a larger share of statistically significant grid points solely due to domain selection. We analyze the origin of this behavior from a rank-based perspective and discuss its implications for spatial inference and uncertainty quantification in environmental sciences.

Based on these insights, we propose practical recommendations for robust and transparent significance assessment, such as spatially aggregated or spatially aware alternatives. Our results highlight both the need to account for multiple-testing and potential issues with a naïve application and interpretation of FDR correction. While illustrated using atmospheric data, the findings are directly relevant to hydrology and other environmental sciences where statistical significance is assessed across spatial fields.

How to cite: Schutte, M., Olivetti, L., and Messori, G.: Which grid points are statistically significant? Revisiting false discovery rate correction in geospatial data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5236, https://doi.org/10.5194/egusphere-egu26-5236, 2026.

EGU26-7544 | ECS | Posters on site | HS3.4

Toward Stable Groundwater–Surface Water Coupling in Landscape Evolution Models 

Farshid Alizadeh, Raphael Bunel, Nicolas Lecoq, and Yoann Copard

Integrated landscape-evolution models require groundwater models that are computationally efficient, groundwater component that remains stable over multidecadal simulations, and strong coupling with surface hydraulics and sediment transport. In CLiDE, which is built on CAESAR–Lisflood, the backward-Euler groundwater update is simple, but as grid resolution or hydraulic diffusivity increases, it becomes highly restrictive due to the diffusion-type Courant–Friedrichs–Lewy (CFL) stability constraint. We present a redesign of CLiDE’s groundwater module that provides two complementary pathways: a behavior-preserving optimized explicit solver and a fully implicit formulation based on backward-Euler time integration. The implicit approach uses a Picard iteration to address the nonlinearity of unconfined transmissivity and the sparse symmetric positive-definite systems with a preconditioned conjugate-gradient solver. We benchmark both solvers across 25 years in fully coupled hydro-geomorphic experiments at the 104 km² Orgeval catchment in north-central France using hourly and daily groundwater coupling intervals. The implicit solver achieves a water mass balance at the catchment scale within 0.1% while remaining unconditionally stable at daily time steps and achieving solutions comparable to the hourly implicit solution. Groundwater head diagnostics are typically within 0.01 m of each other. The consistency in outlet hydrographs, inundation patterns, and long-term sediment-export behavior indicates that daily implicit coupling, in this case, can be selected based on process time scales, and not on numerical stability. Moreover, the optimized explicit solver accelerates the legacy scheme by 1.3 to 1.6 times refinements to specific algorithms, with no change in numerical outputs. Collectively, these advances enhance CLiDE's capability for additional fully coupled, long-duration simulations and suggest a preference between efficiency-oriented explicit updates and robustness-oriented implicit integration.

How to cite: Alizadeh, F., Bunel, R., Lecoq, N., and Copard, Y.: Toward Stable Groundwater–Surface Water Coupling in Landscape Evolution Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7544, https://doi.org/10.5194/egusphere-egu26-7544, 2026.

EGU26-7835 | ECS | Orals | HS3.4

Reliable Predictive Resolution in GeospatialModelling 

Meng Lu and Jiong Wang

High-resolution geospatial prediction and satellite image downscaling are increasingly enabled by advances in machine learning and the availability of fine-scale covariates. However, predicted maps are often delivered on arbitrary grids that are not justified by the sampling density of observations. While uncertainty can be quantified at unobserved locations, the spatial scales over which predictions are supported by the data and the modelling process are typically not characterized. Besides computational and storage costs, critical consequences including over-interpretation, modelling noise, and most importantly, the apparent predictive resolution of spatial products can be misleading for downstream applications, potentially affecting scientific conclusions. An example is the use of predicted air pollution maps in health cohort studies to assess exposure–response relationships. This raises a fundamental but under-addressed question: what is the finest spatial resolution at which predictions are meaningfully supported by the data (and model)?

We investigate how to meaningfully determine the predictive resolution in regression models by linking sampling density and model parameters in the frequency domain through spectral analysis. Two challenges are 1) to identify the sampling density in the multi-dimensional feature space, where the sampling typically becomes irregular; and 2) how to relate the frequency in the feature space to the spatial resolution. Using simulated and real-world geospatial datasets, we show that some arbitrarily selected output resolutions in existing literatures could exceed the data-supported predictive resolution, and could induce unnoticed biases or change-of-support issues in downstream analyses.

How to cite: Lu, M. and Wang, J.: Reliable Predictive Resolution in GeospatialModelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7835, https://doi.org/10.5194/egusphere-egu26-7835, 2026.

Stochastic rainfall models are probabilistic tools able to simulate synthetic rainfall datasets with statistical properties that resemble those from observations, which makes them particularly suitable to assess the uncertainty of rainfall estimates and to conduct sensitivity analysis of hydro-meteorological modeling chains. When the focus of the modeling is on spatial and temporal patterns, models based on space-time Gaussian random fields (GRFs) are often used because they enable modeling rainfall at any point of the space-time domain from sparse and heterogeneous data (typically observations from a rain gauge network).

In this presentation I will explore how a new model of space-time, multivariate and non-stationary GRF can be leveraged to improve stochastic rainfall modeling. A parametric transform function is combined with the GRF to account for rainfall intermittency and skewed marginal distribution, which results in a so-called trans-Gaussian (or meta-Gaussian) model. Among the many applications achieved by this flexible trans-Gaussian model I will examine how spatial non-stationarity can model orographic effects, and how multivariate modeling can be used to embed rainfall into a stochastic weather generator including five different variables (rainfall, temperature, wind, solar radiation and humidity).

How to cite: Benoit, L.: Stochastic rainfall modeling using spatio-temporal, multivariate and nonstationary trans-Gaussian random fields, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7961, https://doi.org/10.5194/egusphere-egu26-7961, 2026.

EGU26-9994 | ECS | Posters on site | HS3.4

Probabilistic mapping of groundwater nitrate pollution using a Bayesian Gaussian process model 

Kassandra Jensch, Márk Somogyvári, and Tobias Krüger

Nitrate groundwater pollution threatens the quality of drinking water and is directly linked to intensive fertiliser inputs on agricultural fields. To reduce pollution from agricultural sources, areas with, or at risk of, elevated nitrate concentrations must be designated as Nitrate Vulnerable Zones (NVZs) under the European Nitrates Directive. In Germany, as elsewhere in Europe, the designation of NVZs follows a binary classification scheme that does not account for uncertainties in the underlying data and interpolation method. We present an alternative geostatistical framework that explicitly introduces uncertainties into the established designation framework, enabling a more accurate assessment of nitrate groundwater pollution. Using a Bayesian Gaussian process model, nitrate concentrations in groundwater were predicted across the federal state of Brandenburg, Germany, where nitrate pollution is an acute problem. Our model specifically incorporates measurement errors as well as systematic biases from different observation types. The model allows for the calculation of exceedance probabilities which provides a continuous representation of nitrate pollution risk across space, relative to the legal nitrate limit of 50 mg/L. We show that the majority of agricultural land in the study area has at least a 50% probability of exceeding this limit. Additionally, measurement errors were identified as the main source of uncertainty in estimated nitrate concentrations, leading to relatively wide posterior predictive distributions. The results indicate that areas with high exceedance probability extend beyond currently designated NVZs. Unlike the established designation workflow, the proposed approach accounts for the complex reality and uncertainty of nitrate pollution in groundwater and can be readily extended to other countries in the EU and beyond. This enables a more robust and transparent designation of NVZs, and demonstrates the value of explicitly incorporating uncertainty into environmental modelling in high-profile policy settings.

How to cite: Jensch, K., Somogyvári, M., and Krüger, T.: Probabilistic mapping of groundwater nitrate pollution using a Bayesian Gaussian process model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9994, https://doi.org/10.5194/egusphere-egu26-9994, 2026.

EGU26-12514 | ECS | Orals | HS3.4

How environmental conditions influence satellite detection of rainfall events 

Chun Zhou, Li Zhou, Luca Brocca, and Dui Huang

Precipitation serves as a critical link between climate and hydrology, with variability shaped by environmental factors that regulate satellite detection under complex conditions. Physical response mechanisms under varying temperature, soil moisture, and pressure remain insufficiently assessed. Using global gauge precipitation and ERA5-Land reanalysis data, we identified HIT, MISS, FALSE events and examined their differential responses to key environmental variables. We demonstrate that HIT events tend to occur under intermediate environmental conditions, with both products sharing similar responses but GSMaP exhibiting slightly smoother temperature signals and IMERG stronger soil-moisture-related variability. MISS events, linked to colder, wetter backgrounds, are associated with larger spread, while FALSE events arise mainly in warm, dry regimes with low soil moisture and more fluctuations in IMERG. Environmental factors modulate detection, with warmer and wetter conditions favoring HIT and suppressing FALSE, while pressure plays a weaker, secondary role. These findings support satellite-based global hydrology and climate-resilience assessment.

How to cite: Zhou, C., Zhou, L., Brocca, L., and Huang, D.: How environmental conditions influence satellite detection of rainfall events, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12514, https://doi.org/10.5194/egusphere-egu26-12514, 2026.

EGU26-13518 | Orals | HS3.4

Trend or persistence: what are we really detecting in annual low-flow time series? 

Gregor Laaha and Johannes Laimighofer

Trends in annual low-flow time series are central to water resources and drought management, yet estimates are strongly affected by serial persistence, and dependence can make persistence appear as trend. We compare nonparametric and parametric methods under short-term autocorrelation and long-term persistence (LTP) and evaluate their reliability with European streamflow data and simulation-based experiments.

For short-term autocorrelation, modified Mann–Kendall approaches with block-bootstrap-based significance correction (BBSMK) and simultaneous bias-corrected prewhitening yield robust results; alternative variants inflate significance and produce implausible findings. Parametric ARIMAX models indicate that, when analyses are based on the water year, only a small share of series require higher autoregressive orders, whereas calendar-year aggregation induces more complex correlation structures and, in turn, unreliable (too low) significance rates.

Under long-term dependence, the nonparametric Mann–Kendall–LTP approach markedly lowers the fraction of significant trends, while FARIMAX models (external trend + LTP) produce similar rates to BBSMK. Yet AIC-based selection typically replaces LTP with short-term autocorrelation, indicating that what appears as persistence is often explainable by short-range dependence.

We finally assess misclassification in parametric and nonparametric trend models under LTP using nature-based simulations across record lengths. Calibrated to stream-gauge records, the simulations test whether series with deterministic trends and short-term autocorrelation—but without true LTP—are misclassified as LTP, and how such misclassification biases trend estimates. Across four scenarios (high/low LTP × significant/non-significant trend), LTP misclassification and trend-detection errors are elevated: with a trend present, short-term autocorrelation is often mistaken for LTP, biasing estimates and reducing power. At hydrologically typical record lengths, errors remain substantial, declining only for extremely long series (1,000–10,000 years); misclassification of short-term correlation as LTP persists even then.

Overall, under common record lengths and dependence structures, deterministic trends are often misinterpreted as long-term persistence—and, conversely, genuine persistence can be mistaken for trend. Therefore, LTP-based trend analyses should be interpreted with caution; typical hydrological records are too short for reliable LTP inference.

How to cite: Laaha, G. and Laimighofer, J.: Trend or persistence: what are we really detecting in annual low-flow time series?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13518, https://doi.org/10.5194/egusphere-egu26-13518, 2026.

This study investigates multilevel flood susceptibility mapping at the national scale in North Macedonia, utilizing 328 historical flood events, 14 conditioning factors derived from a digital elevation model, simplified lithology, and computed direct runoff. The methodology integrates fuzzy set theory (Fuzzy), analytic hierarchy process (AHP), weighted linear combination (WLC), and random forest (RF) approaches. The two-stage process employs distinct sets of conditioning factors in sequential flood susceptibility mapping: first, generating Fuzzy/AHP/WLC predictions and pseudo-absence data, and second, producing five RF predictions by varying pseudo-absences and binary cutoffs. Validation results indicate that the very high susceptibility class (0.8–1.0) of the Fuzzy/AHP/WLC model predicted 46.6% of flood pixels within 31.6% of the total area. In comparison, the very high susceptibility class of the RF models predicted 88.5%, 78.3%, 60.6%, 48.5%, and 28.3% of flood pixels within 54.7%, 42.2%, 30.5%, 27.0%, and 25.1% of the total area, respectively. The RF models achieved area under the curve (AUC) values exceeding 0.850, with a maximum of 0.966. Furthermore, a standard deviation map derived from the RF models identified regions of high and low uncertainty, highlighting areas for potential methodological improvement and targeted sampling. The results also show the promise of the multilevel approach for mapping flood susceptibility and call for more research into its potential for future studies and real-world applications.

How to cite: Gorsevski, P. and Milevski, I.: Multilevel flood susceptibility mapping by fuzzy sets, analytical hierarchy process, weighted linear combination and random forest, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14278, https://doi.org/10.5194/egusphere-egu26-14278, 2026.

Spatial statistics provides a principled framework for analyzing environmental variables that exhibit spatial dependence, enabling inference and prediction in systems governed by heterogeneous processes. In many hydrogeological applications, the most informative perspective emerges from fusing complementary datasets, for example, sparse groundwater observations and spatially exhaustive remote sensing products. This data fusion is rarely straightforward because data sources often differ in sampling design, uncertainty, and, crucially, spatial support (the area or footprint represented by a measurement). When observations collected at one support are used to predict at another, the change-of-support problem can induce biased variances and degraded predictions if scale effects are ignored. Here, we integrate groundwater levels from a monitoring network with multi-resolution remote sensing covariates to improve groundwater depth mapping while explicitly accounting for support differences. The study targets groundwater level prediction in Southeast Brazil, where relief compartments and land-use patterns generate strong spatial heterogeneity in recharge and water consumption. We combine in situ groundwater table depths observed at 56 monitoring locations with (i) geomorphological information derived from the 30 m TanDEM‑X dataset and (ii) land-surface water consumption represented by 10 m evapotranspiration estimates from SAFER (Simple Algorithm for Evapotranspiration Retrieving). These covariates encode terrain-driven controls and land-use effects that are not fully captured by point measurements alone. Spatial dependence within and across variables is modeled using the Linear Model of Coregionalization (LMC), enabling coherent estimation of direct and cross-variograms. To ensure consistency across supports, we address support homogenization by regularizing point-support variances and cross-structures to a common block support defined on the prediction grid. This regularized LMC is then used within a collocated block cokriging (CBCK) framework, which applies collocated block covariates to enhance block-scale groundwater predictions. Model performance demonstrates substantial gains from explicitly treating change of support and incorporating multi-resolution covariates. CBCK yields reliable groundwater depth predictions with root mean squared error (RMSE) of 0.41 m, markedly outperforming ordinary block kriging (OBK) estimations (RMSE = 2.89 m) and improving upon prior CBCK implementations that relied on coarser (500 m) evapotranspiration inputs (RMSE = 0.49 m). Beyond accuracy improvements, the resulting maps better reflect the coupling between land-use water demand, terrain-driven controls, and groundwater levels, supporting groundwater management decisions relevant to agronomic planning and ecosystem sustainability. The proposed methodology is transferable to other aquifer systems and can be adapted to alternative remote sensing products and field measurements to explore climate, land use, and hydrogeology interactions across spatial scales.

How to cite: Lilla Manzione, R. and de Oliveira Ferreira Silva, C.: Multi-source data fusion to enhance groundwater levels prediction: merging monitoring networks and orbital remote sensing datasets, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22108, https://doi.org/10.5194/egusphere-egu26-22108, 2026.

NP3 – Scales, Scaling and Nonlinear Variability

This study investigated the complex temporal behavior of cosmogenic Beryllium-7 (7Be) by analyzing daily activity concentrations from 21 monitoring stations in the CTBTO network, spanning the years 2010 through 2017. By applying multifractal detrended fluctuation analysis (MF-DFA), it was established that 7Be time series exhibit significant nonlinear scaling behaviors. The results indicate a broad multifractal spectrum (Δα ranging from 0.17 to 0.66), with statistically significant multifractality observed at all locations except RN45 and RN47. Leveraging the extracted spectral width and Hölder exponents, current study utilized the K-means algorithm to categorize the global stations into three distinct clusters based on their dynamic signatures. Furthermore, this study assessed the external forcing of 7Be variations via multifractal cross-correlation analysis against five major indices: the Southern Oscillation Index (SOI), North Atlantic Oscillation (NAO), and solar activity markers (Total, Northern, and Southern hemisphere sunspot numbers). While cross-correlations varied across indices, the NAO emerged as the dominant driver. Notably, station RN16 (Yellowknife, Canada) displayed the highest sensitivity to these external drivers, suggesting a unique coupling between atmospheric/solar indices and isotope concentration at this latitude.

How to cite: Ogunjo, S.: Global Beryllium-7 Dynamics: Nonlinear Scaling Properties, Spatial Classification, and Sensitivity to Atmospheric Teleconnections, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-963, https://doi.org/10.5194/egusphere-egu26-963, 2026.

Various empirical methods exist to calculate fractal dimension of geospatial objects with the box-counting principle being a popular one. However, these methods generally require geospatial data to be projected to Euclidean space. While this works fine at small geographic scales, computation at larger or global scales introduces distortions inevitable with projection due to the curvature of the earth. I show from mathematical principles how Discrete Global Grid Systems (DGGSs) – hierarchical spatial data structures composed of polygonal cells that are increasingly being used for modelling geospatial data – can be employed creatively to act as the covering set for calculating the Minkowski-Bouligand dimension using the box-counting principle. This enables computation of the fractal dimension of geospatial data in spherical coordinates without having to project the data in question on a planar surface. Results on synthetic datasets are within 1% of their theoretical fractal dimensions. A case study on opaque cloud fields obtained from a geostationary meteorological remote sensing satellite image yields a result of 1.577±0.0207 when aggregated using three different geodesic DGGSs based on the Icosahedral Snyder Equal Area (ISEA) projection, in line with values reported in the literature. As the cells of a DGGS are generally pre-defined and fixed to the earth, this method also brings some relief associated with the box-counting method in general, particularly the choice of cell-sizes to be sampled as well as the placement and orientation of the grid that acts as the covering set – issues that are usually circumvented by rules of thumb and conventions. I comment on the possibility to extend the method for use with raster data.  Ways to improve the method using low-aperture DGGSs to better capture the self-similarity and possibilities of developing custom DGGSs for this purpose are also noted. Being a computationally intensive method, development of software libraries making use of parallel computing to enhance performance and scalability is also proposed. With climatic variables exhibiting spatiotemporal autocorrelation with long-range effects, I believe this method would be of interest to climate scientists interested in studying their fractal properties at continental and global scales.

How to cite: Ghosh, P.: Computing fractal dimension at large geographic scales using Discrete Global Grid Systems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4299, https://doi.org/10.5194/egusphere-egu26-4299, 2026.

EGU26-4711 | ECS | Orals | NP3.3

Numerical Study on the Path-Dependent Evolution of the Excavation Damage Zone under Transient Unloading 

Gongliang Xiang, Ming Tao, Xibing Li, Qi Zhao, Linqi Huang, Tubing Yin, Rui Zhao, and Jiangzhan Chen

Excavation and unloading of deep rock mass under varying in-situ stress levels is a typical non-linear geomechanical process, Specifically, in the context of the widely used drilling and blasting (D&B) method, the excavation damage zone (EDZ) around underground opening induced by transient unloading represents a dynamic response problem governed by multiple factors. While the exact theoretical solution of stress state in surrounding rock during transient excavation can describe the stress state and eventually converge to the Kirsch solution after rock mass excavation completed, it cannot fully capture the dynamic damage process. Therefore, a circular tunnel model for transient excavation was established in this study using a dynamic finite element code LS-DYNA. An equivalent released nodal force method was implemented to stably control the transient unloading path under non-hydrostatic in-situ stress conditions after stress initiation, which realizing the synchronous release of radial and tangential stresses in the excavated zone. Moreover, the validity of the linear elastic transient excavation model was verified through comparison with an analytical solution. Then the dynamic stress redistribution, as well as the EDZ evolution process were numerically simulated under various stress unloading paths and lateral pressure coefficients, utilizing an elastoplastic constitutive model. This study provides a basis for simulating transient excavation under various paths and understanding failure of surrounding rock in non-hydrostatic stress states.

How to cite: Xiang, G., Tao, M., Li, X., Zhao, Q., Huang, L., Yin, T., Zhao, R., and Chen, J.: Numerical Study on the Path-Dependent Evolution of the Excavation Damage Zone under Transient Unloading, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4711, https://doi.org/10.5194/egusphere-egu26-4711, 2026.

EGU26-7074 | Posters on site | NP3.3

Global-scale multidecadal climate variability: The stadium wave 

Sergey Kravtsov, Andrew Westgate, and Andrei Gavrilov

A significant fraction of multidecadal fluctuations in the reanalysis-based gridded estimates of the observed climate variability over the past century and a half lie outside of the envelope generated by ensembles of climate-model historical simulations. Several pattern-recognition methods have been previously used to map out a truly global reach of the observed vs. simulated climate-data differences; in our own work we dubbed these global discrepancies the stadium wave to highlight their most striking spatiotemporal characteristic. Here we used a novel combination of such methods in conjunction with a large multi-model ensemble and two popular twentieth-century reanalysis products to: (i) succinctly describe the geographical evolution of the observed stadium wave in the annually sampled near-surface atmospheric temperature and mean sea-level pressure fields in terms of three basic patterns; (ii) show the robustness of this identification with respect to methodological details, including the demonstration of the truly global character of the stadium wave; and (iii) provide essential clues to its dynamical origin. All input time series were first decomposed into the forced signal and the residual internal variability; multi-model forced-signal estimates were also decomposed into their common-evolution part and the individual-model residuals. Analysis of the latter residuals suggests a contribution to the stadium-wave dynamics from a delayed climate response to variable external forcing despite the observed stadium-wave patterns’ exhibiting the magnitudes and the level of global teleconnectivity unmatched by the forced-signal residuals.

How to cite: Kravtsov, S., Westgate, A., and Gavrilov, A.: Global-scale multidecadal climate variability: The stadium wave, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7074, https://doi.org/10.5194/egusphere-egu26-7074, 2026.

Scaling dynamics, intermittency, and multifractality in complex natural systems remain a central challenge across physics, geoscience, and hazard science. Earth system dynamics exhibit strongly non-equilibrium behaviour, long-range codependences, irreversible energy and information flows, and multiscale spatiotemporal coevolution, including dynamically adaptive interactions across spatial, temporal, and organizational domains.

The present contribution introduces and explores our latest advances in information physical intelligence for addressing these challenges, further building from our recent developments in non-ergodic nonlinear open quantum systems, where systems non-recurrently exchange energy, matter and information with structural-functional coevolutionary environments. In this setting, entropy production, information backflow, coherence, and decoherence are anchored on cross-scaling organizing principles spanning from microphysical foundations to emergent macrophysical behaviour, dynamically traceable and solvable through our novel nonlinear quantum developments.

Our new nonlinear quantum intelligence framework is then equipped with our latest non-ergodic information physical categorical algebraic infrastructure and associated mathematical physics apparatus, underlying the natural emergence of coevolutionary cyber-physical cognitive systems. These are then tested in controlled synthetic and free-range natural experiments, in order to provide operational insights on their ability to autonomously unfold and shape structural-functional emergence of complex system dynamics including scaling mechanisms in nonlinear non-ergodic multiscale stochastic-dynamical systems exhibiting scale-dependent entropy production rates, anomalous dissipation, and multidirectional cascades, on an inherent information physical thermodynamic process for far-from-equilibrium coevolutionary multifractal scaling.

One of the advances herein brings out a novel coevolutionary far-from-equilibrium thermodynamic renormalization of non-ergodic open quantum dynamics, where delocalization and aggregation across scales induces effective non-Markovianity, memory kernels, and scale-dependent effective energetics. These features are then shown to map naturally onto formal multifractal signatures observed in turbulence, precipitation fields, seismicity, geomagnetic activity, and climate variability.

Within this framework, coevolutionary multifractality emerges as a signature of competing irreversible processes operating across coevolving subsystems, rather than as a purely statistical or kinematic geometric construct. The corresponding generalization of information-theoretic quantities, including quantum relative entropy, Fisher information, and entropy production fluctuations, provide structural descriptors of scaling regimes and phase-transition-like behaviour in Earth system dynamics.

From theory to operation, we demonstrate how these information physical foundations and developments enable cross-domain integration in multiscale, multidomain Earth system modeling and more broadly across our System-of-Systems for Multi-Hazard Risk Intelligence Networks (SoS4MHRIN) platform. In doing so, we unveil and elicit coevolutionary scaling mechanisms linking traditional quantum information to meso and macroscale complexity, and harness elusive predictability pertaining to far-from-equilibrium non-ergodic non-recurrent emergence, intermittence and persistence of structural-functional changes, critical transitions and extreme events, along with their interactions and impacts.

This is particularly relevant for compound, cascading, coevolutionary and synergistic multi-hazards, where earthquakes, volcanic eruptions, extreme weather, floods, wildfires, and landslides interact across scales and domains. Far-from-equilibrium entropy production and information physical flows act as early warning indicators and organizing variables for multi-hazard interactions and tipping dynamics.

By synergistically articulating non-ergodic information physics, nonlinear open quantum thermodynamics, scaling theory, and Earth system science, this work provides a physically grounded, scale-aware framework for better understanding and operating on complexity, predictability, and resilience in the Earth system under ongoing structural-functional multiscale coevolution.

 

How to cite: Perdigão, R. A. P. and Hall, J.: Nonlinear Quantum Intelligence Framework for Coevolutionary Scaling and Multifractality across Far-from-Equilibrium Earth System Dynamics and Multi-Hazards, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7773, https://doi.org/10.5194/egusphere-egu26-7773, 2026.

EGU26-8215 | ECS | Orals | NP3.3

Accounting for spatially autocorrelated errors is necessary to infer cross-scale biodiversity–ecosystem functioning patterns in natural world 

Zibo Wang, Yunfei Li, Fen Zhang, Jianye Yu, Chongshan Wang, Long Chen, and Xiaohua Gou

Cross-scale biodiversity–ecosystem functioning (BEF) relationships are widely used to evaluate how biodiversity relates to ecosystem functioning across space. Theory predicts that when species turnover is incomplete across space, the BEF slope follows a characteristic hump-shaped scaling pattern, strengthening with increasing scale before weakening at broader scales. In real landscapes, however, biodiversity and ecosystem function often co-vary along environmental gradients, and spatial autocorrelation naturally increases with scale, potentially confounding regression-based BEF inference.

We combined simulations and field data to quantify how explicitly accounting for spatial autocorrelation (SAC) affects BEF scaling. In simulations, biodiversity and ecosystem function were generated under joint control of an environmental gradient and a spatial stochastic component, allowing SAC to emerge in both predictors and responses. In empirical analyses, we used forest inventory data from two temperate forests. We constructed a sequence of spatial scales by aggregating plots using a k-nearest-neighbor procedure, with k increasing from small to large neighborhoods. At each scale, we estimated BEF as the slope of species richness (SR) on biomass increment, while controlling for climate, soil, and trait covariates. We then contrasted non-spatial models with spatial models that include SAC in the residual structure, and quantified ΔBEF as the difference in SR slopes between spatial and non-spatial fits.

Across simulations and observations, ignoring SAC produced an apparently monotonic strengthening of BEF with scale. However, when SAC was included, the BEF scaling curve followed the predicted hump-shaped pattern. Moreover, ΔBEF increased with residual Moran’s I, indicating that stronger spatial dependence systematically inflates non-spatial BEF estimates as scale increases. Finally, the BEF slopes were negatively correlated with excess species richness and positively correlated with species turnover after correcting for SAC, consistent with the theory that species turnover plays a key role in BEF scaling. Our study emphasizes that accounting for SAC is essential for accurate BEF scaling and provides a useful approach for future studies.

How to cite: Wang, Z., Li, Y., Zhang, F., Yu, J., Wang, C., Chen, L., and Gou, X.: Accounting for spatially autocorrelated errors is necessary to infer cross-scale biodiversity–ecosystem functioning patterns in natural world, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8215, https://doi.org/10.5194/egusphere-egu26-8215, 2026.

EGU26-9513 | ECS | Posters on site | NP3.3

CMIP6 simulations overestimate historical decadal temperature variability over most land areas 

Tom Schürmann and Kira Rehfeld

A robust understanding of the potential range of Earth system dynamics is essential for effectively simulating future climate change. Previous studies have reported increasing discrepancies in modelled temperature variability from global to local scale, and beyond decadal timescales, based on paleoclimate reconstructions. The instrumental record is most complete for the last 145 years. This limits a spatio-temporal assessment of historical temperature variability to multidecadal timescales at the upper end.  To this day, model-observation comparisons of regional climate variability have mostly focused on sea surface temperature. 

Here, we compare historical near-surface air temperatures from an ensemble of 50 CMIP6 models with similar initial conditions and two single-model initial-condition large ensembles (SMILE) with reanalysis and observation datasets. Following a robust like-for-like approach, all datasets are interpolated to a common grid of about 2.8 degrees and compared over the period of 1880 to 2015. Spectral analysis and filters reveal the structure of temperature variability over different spatial and temporal scales. Specifically, we focus on temperature variability on timescales of 10 to 30 years from global to local scale.  

On the global scale, models consistently display higher temperature variance in bands from 10 to 30 years than reanalysis data. Masking the analysis to regions with a consistent observational record confirms this trend. On the local scale, observed temperature variability can deviate substantially from the mean of stacked model standard deviation fields. For example, observed temperature variability in Europe lies in the lower tail of the model distribution. Vice versa, observed temperature in the southern Atlantic is representative of the model distributions' upper tail. Consistently over the multi-model ensemble and two SMILEs, decadal temperature variability is overestimated on land, but underestimated over the ocean. Nevertheless, there are exceptions to this pattern. For example, in the northern Atlantic, modelled variability overestimates observations consistent with the literature. Overall, these regional inconsistencies suggest that multiple, regionally heterogeneous processes are involved. 

How to cite: Schürmann, T. and Rehfeld, K.: CMIP6 simulations overestimate historical decadal temperature variability over most land areas, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9513, https://doi.org/10.5194/egusphere-egu26-9513, 2026.

Empirical, data-driven models provide a complementary approach to dynamical models for simulating and forecasting weather and climate variability across daily to subseasonal timescales. We present ongoing work toward the development of a global, data-driven weather emulator for temperature and precipitation based on higher-order Linear Inverse Models (LIMs) formulated within the Empirical Model Reduction (EMR) framework. This formulation enables the representation of effective low-order dynamics, memory effects, and scale-dependent variability embedded in high-dimensional atmospheric fields. Rather than relying on a fixed EOF-based spatial decomposition, we explore a state-space approach in which the spatial basis is parameterized and optimized using Kalman filtering, thereby learning an optimal dynamical representation directly from the data.

The model is trained using a combination of NASA satellite observations and atmospheric reanalysis products. Near-surface temperature is modeled directly, while precipitation is represented using a pseudo-precipitation variable: precipitation equals observed rainfall where it occurs and otherwise corresponds to the negative air-column integrated water-vapor saturation deficit, defined as the amount of water vapor required to bring the atmospheric column to saturation at each vertical level. This formulation yields a continuous and dynamically meaningful representation of moist processes that facilitates the analysis of variability statistics across scales.

Model performance is evaluated in terms of its ability to reproduce observed variability statistics, temporal persistence, and subseasonal prediction skill, while dynamical diagnostics will be used to investigate the underlying sources of forecast skill. By focusing on the statistical and dynamical representation of variability, this work contributes to ongoing efforts to bridge data-driven modeling and theoretical perspectives on weather to climate variability across scales.

How to cite: Hébert, R. and Kravtsov, S.: A Global Data-Driven Weather Emulator for Temperature and Precipitation Based on Higher-Order Linear Inverse Modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10397, https://doi.org/10.5194/egusphere-egu26-10397, 2026.

EGU26-11706 | ECS | Posters on site | NP3.3

Atlantic Multidecadal Variability-like behaviour since 1850 is largely externally forced 

Yongyao Liang, Ed Hawkins, Gerard McCarthy, and Peter Thorne

Whether observed Atlantic Multidecadal variability (AMV) is truly an intrinsic internal mode of climate variability or an externally forced response remains contentious, with conflicting literature that North Atlantic SST variability arises from internal dynamics or external forcing. The availability of several single-model initial-condition large ensembles (SMILEs) and new insights into potential biases in sea surface temperature (SST) variations offer a fresh opportunity to reassess this question. We show that SMILE ensembles provide strong evidence that AMV-like variability is largely externally forced. New insights into potential SST biases also raise questions about apparent early 20th-century oscillatory behaviour, suggesting that discrepancies between observations and climate model simulations may not arise solely from model deficiencies. SMILE models with stronger multidecadal variability show weaker agreement with observed AMV phasing, even in the best-performing individual ensemble members, suggesting that large internal model variability may obscure the forced signal. We conclude that future variations in North Atlantic SST will very likely be driven primarily by future anthropogenic activities.

How to cite: Liang, Y., Hawkins, E., McCarthy, G., and Thorne, P.: Atlantic Multidecadal Variability-like behaviour since 1850 is largely externally forced, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11706, https://doi.org/10.5194/egusphere-egu26-11706, 2026.

EGU26-12081 | ECS | Posters on site | NP3.3

Universal Multifractals characterization of high-resolution rainfall in the Paris region 

Atheeswaran Balamurugan, Auguste Gires, Daniel Schertzer, and Ioulia Tchiguirinskaia

Rainfall exhibits strong variability, intermittency and a heavy-tailed distributions across a wide range of scales. Understanding and characterizing these features is needed for numerous applications such as quantifying the extremes or merging measurements from various sensors operating at different space-time scales. 

This study presents a comprehensive multifractal analysis of high-resolution (30 s) 1D rainfall time series from the Paris region (2018 – 2024) using the Universal Multifractals (UM) framework. The data was collected with the help of optical disdrometers installed on the campus of Ecole nationale des Ponts et chausséee campus (https://hmco.enpc.fr/portfolio-archive/taranis-observatory/) UM framework has been widely used to characterize and simulate rainfall across wide range of scales with the help of only three parameters: the mean intermittency C₁, the multifractality index α and  the non-conservation parameter H. 

Spectral analysis identifies a clear scale break around 1 h, separating two distinct regimes. Coarse scales (>1h) are characterized by smooth, low-intermittency variability (spectral slope β ≈ 0.4), while fine scales (<1h) exhibit stronger spectral slope (β > 1). Accordingly, a regime-dependent analysis strategy is adopted: actual rainfall series are used at coarse scales to preserve large scale structure, while absolute values of fluctuation series are preferred at fine scales to reduce to study underlying conservative field and obtain cleaner scaling behaviour.

Analyses reveal strong multifractality (α ≈ 1.6 –1.7) and moderate intermittency (C₁ ≈ 0.12 – 0.45) at fine scale regimes. At coarser scale regimes, rainfall exhibits smoother variability with moderate multifractality (α < 1)and lower intermittency (C₁ ≈ 0.15–0.18). The UM parameters display good inter annual stability over 2018 – 2024, mild seasonal modulation (slightly higher C₁ in summer), and individual rain-event analyses were performed to examine event-to-event variability, indicating substantial heterogeneity between events.  

These results demonstrate the relevance of the UM framework for quantitatively characterizing rainfall variability in the Paris region. Initial attempts to interpret the observed differences between fine and coarse scales regimes using a unique model will be presented. 

Authors acknowledge partial financial support by the European Union as part of the Horizon Europe programme, Marie Skłodowska-Curie Actions, call COFUND-2022 and under grant agreement number 101126720; the France-Taiwan Ra2DW project (grant number by the French National Research Agency – ANR-23-CE01-0019-01).

How to cite: Balamurugan, A., Gires, A., Schertzer, D., and Tchiguirinskaia, I.: Universal Multifractals characterization of high-resolution rainfall in the Paris region, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12081, https://doi.org/10.5194/egusphere-egu26-12081, 2026.

EGU26-12716 | ECS | Posters on site | NP3.3

Linking meteorological extremes to clay shrink–swell hazard: Insights from 65 years of climate data 

Carl Tixier, Pierre-Antoine Versini, and Benjamin Dardé

Clay shrink-swell (CSS) behavior arises from fluctuations in soil moisture driven by seasonal cycles of rainfall and drought. This phenomenon causes ground movements that can damage building foundations and infrastructure. In France, where approximately 54% of constructions are exposed to this hazard, CSS ranks as the second most significant category of natural disaster insurance claims.

The French central reinsurance fund reports that the average annual cost, calculated over a five-year sliding window, remained below €300 million in 2016. Since 2017, this figure has increased, reaching about €1.35 billion as of 2025. Climate change is expected to amplify droughts, heatwaves, and precipitation extremes, further intensifying CSS processes and potentially rendering their financial burden unsustainable for insurers.

To address this issue, we analyze meteorological data from the SAFRAN reanalysis provided by Météo-France, which offers daily observations at an 8 km spatial resolution across France since 1958. Our study applies geostatistical and multifractal techniques to characterize spatiotemporal variability, identify scale breaks, estimate extreme values, and examine spectral properties of key climatic variables. Specifically, we compute:

  • Multifractality index (α): It measures the speed of change in intermittency;
  • Mean singularity (C₁): Average singularity, characterizes intermittency;
  • Maximum probable singularity (γₛ): maximum probable singularity.

Tracking these parameters from 1958 to 2025 enables us to identify regions most affected by changes in extremes. Analyses focus on variables influencing CSS behavior, including precipitation, temperature, evapotranspiration, and soil moisture index.

Finally, we compare the evolution of extremes in these climatic parameters with trends in CSS occurrence, quantified through insurance claims. This spatial and temporal comparison between multifractal indicators and affected areas provides insights into the relationship between the intensification of extreme meteorological events and the dynamics of clay shrink-swell processes.

This work is part of the IRGAK (inhibition of clay shrinkage-swelling by K+ ion injection) project, founded by the French Agency for Ecological Transition (ADEME). Its objective is to model the link between climate variability and CSS, and to propose adaptation strategies to mitigate a risk that is expected to increase significantly with climate change, leading to escalating insurance costs and growing socio-economic impacts.

How to cite: Tixier, C., Versini, P.-A., and Dardé, B.: Linking meteorological extremes to clay shrink–swell hazard: Insights from 65 years of climate data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12716, https://doi.org/10.5194/egusphere-egu26-12716, 2026.

EGU26-14920 | Orals | NP3.3

Understanding extreme heat: Causes and time scales revealed by Rényi information transfer 

Milan Paluš, Pouya Manshour, Anupam Ghosh, Zlata Tabachová, Eva Holtanová, and Jiří Mikšovský

Recently, Paluš et al. (2024) demonstrated that information-theoretic generalization of Granger causality – based on conditional mutual information/transfer entropy – when reformulated in terms of Rényi entropy, provides a time-series analysis tool suitable for identifying the causes of extreme values in affected variables.

Investigating the causes of warm summer surface air temperature extremes in Europe, Rényi information transfer highlights the role of blocking events among large-scale circulation patterns and modes of variability. Soil moisture interacts with air temperature on a daily scale, exhibiting bidirectional causal effects on the mean, whereas its influence on temperature extremes emerges over longer time scales, from a fortnight to a month. In contrast, the causal effect of blocking on temperature extremes is primarily observed at the daily scale. Using tools from Rényi information theory, we aim to disentangle this complex, multicausal, multiscale phenomenon and identify the regions in Europe where these factors modulate the probability of extreme summer heat.

 

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 Science Foundation, Project No. 25-18105S.

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., Manshour, P., Ghosh, A., Tabachová, Z., Holtanová, E., and Mikšovský, J.: Understanding extreme heat: Causes and time scales revealed by Rényi information transfer, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14920, https://doi.org/10.5194/egusphere-egu26-14920, 2026.

EGU26-14999 | Orals | NP3.3

From Eons to Epochs: multifractal  Geological Time and a compound multifractal-Poisson model 

Shaun Lovejoy, Andrej Spiridonov, Raphael Hebert, and Fabrice Lambert

Geological time is punctuated by events that define biostrata and the Geological Time Scale’s (GTS) hierarchy of eons, eras, periods, epochs, ages. Paleotemperatures and macroevolution rates, have already indicated that the range ≈ 1 Myr to (at least) several hundred Myrs) is a scaling (hence hierarchical) “megaclimate” regime.  We apply analysis techniques including Haar fluctuations, structure functions trace moment and extended self-similarity to the temporal density of the boundary events (r(t)) of two global and four zonal series.  We show that r(t) itself is a new paleoindicator and we determine the fundamental multifractal exponents characterizing the mean fluctuations, the intermittency and the degree of multifractality.  The strong intermittency allows us to show that the (largest) megaclimate  scale is at least  ≈ 0.5 Gyr.  We also analyze a Precambrian series going back 3.4Gyrs directly confirming this limit and allowing us to quantatively compare the Phanerozoic with the Proterozoic eons.

We find that the probability distribution of the intervals (“gaps”) between boundaries and find that its tail is also scaling with an exponent qD≈ 3.3 indicating huge variability with occasional very large gaps such that it’s third order statistical moment barely converges.  The scaling in time implies that record incompleteness increases with its resolution (the “Resolution Sadler effect”), while scaling in probability space implies that incompleteness increases with sample length (the “Length Sadler effect”). 

The density description of event boundaries is only a useful characterization over time intervals long enough for there to be typically one or more events.  In order to model the full range of scales (and low to high r(t)), we introduce a compound Poisson-multifractal model in which the multifractal process determines the probability of a Poisson event.   The model well reproduces all the observed statistics.

Scaling changes our understanding of life and the planet and it is needed for unbiasing many statistical paleobiological and geological analyses, including unbiasing spectral analysis of the bulk of geodata that are derived from cores.

How to cite: Lovejoy, S., Spiridonov, A., Hebert, R., and Lambert, F.: From Eons to Epochs: multifractal  Geological Time and a compound multifractal-Poisson model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14999, https://doi.org/10.5194/egusphere-egu26-14999, 2026.

EGU26-15166 | ECS | Orals | NP3.3 | Highlight

Global sonde datasets do not support a mesoscale transition in the turbulent energy cascade 

Thomas DeWitt, Tim Garrett, Karlie Rees, and Stephen Oppong

The dynamics driving Earth's weather are commonly presumed to be governed by a hierarchy of distinct dynamical mechanisms, each operating over some limited range of spatial scales. The largest scales are argued to be driven by quasi-two-dimensional turbulence, the mesoscales by gravity waves, and the smallest scales by 3D isotropic turbulence. In principle, such a hierarchy should result in observable breaks in atmospheric kinetic energy spectra at discrete points as one mechanism transitions to the next. Using global radiosonde and dropsonde datasets, we show that this view is not supported in observations. Between 200m and 8km, we find that structure functions calculated along the vertical direction display a Hurst exponent of H_v \approx 0.6, which is inconsistent with either gravity waves (H_v = 1) or 3D turbulence (H_v = 1/3). In the horizontal directions, large-scale structure functions between 200km and 1800km display a Hurst exponent of H_h \approx 0.4, which is inconsistent with quasi-geostrophic dynamics (H_h = 1). We show that these observations are instead consistent with a lesser-known theory of stratified turbulence proposed by Lovejoy and Schertzer in 1985, where at all scales the dynamics obey a single anisotropic turbulent cascade with H_v=3/5 and H_h =1/3.

Our results suggest a reinterpretation of atmospheric dynamics: rather than being controlled by a hierarchy of distinct dynamical elements, atmospheric flow should instead be thought of as a superposition of anisotropic turbulent eddies that continually cascade from large scales to small scales. We show how this view may be interpreted literally and used to construct photorealistic and quantitatively accurate simulations of atmospheric volumes, and without integration of the hydrodynamic equations. We argue that the model also provides a more intuitive basis for interpreting both the intermittent and the anisotropic aspects of the observed statistics of the atmosphere.

How to cite: DeWitt, T., Garrett, T., Rees, K., and Oppong, S.: Global sonde datasets do not support a mesoscale transition in the turbulent energy cascade, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15166, https://doi.org/10.5194/egusphere-egu26-15166, 2026.

The background continuum of climate variability recorded in proxy records is often modelled using parametric spectral models, such as power-laws, auto-regressive processes, or stochastic differential equations.

However, fitting such models to proxy data is usually done in an ad-hoc manner, such as by using least-squares fitting in log-log space.

Here I will discuss two formal Bayesian methods for fitting parametric stochastic models to proxy data. One is a spectral-domain approach based the Whittle likelihood. The other is a time-domain approach based on Gaussian Processes.

In both cases, I show how the standard approaches can be modified to account for some of the ways in which climate proxies alter spectral slopes: measurement error, time uncertainty, uneven sampling, and smoothing (e.g. from diffusion or bioturbation). Finally, I use synthetic data generated from power-law and Matern processes, and proxy-system models, to show expected skill of the two approaches for different proxies.

I find that these formal approaches provide significant bias reduction relative to typical ad-hoc approaches, allowing for much more accurate calibration of stochastic models of climate variability across scales.

How to cite: Proistosescu, C.: Bayesian methods for fitting spectral models to noisy, sparse, proxy data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15967, https://doi.org/10.5194/egusphere-egu26-15967, 2026.

EGU26-19188 | ECS | Orals | NP3.3

New classes of climate model emulators to improve paleoclimate reconstructions 

Auguste Gaudin and Myriam Khodri

It is well known that the predictability of the climate varies over time and will depend on the initial conditions, especially when considering non-linear systems such as El Niño Southern Oscillation (ENSO). While recent decades have seen a few extreme ENSO events, proxy data reveal a large amplitude in tropical Pacific sea surface temperatures low frequency modulations over past millennia. To better interpret what is observed in proxies, a useful approach is to combine the climate information derived from natural archives with the physics of GCMs using paleoclimate data assimilation (PDA). Recently, efficient online ensemble-based data assimilation techniques have been developed relying on climate model emulators and the predictable components of the climate system. The skill of these ensemble forecasts is a key factor for the success of PDA especially when considering Particle Filters. Such predictability may however change according to the host-GCM, the emulator skills in capturing the host-GCM non-linear behaviours and the dimension of the problem. In this study, we explore these issues in a perfect model framework across PMIP3 and PMIP4 climate model simulations for the past millennium, relying on various types of architectures and climate model emulators. Our results indicate that relying on such a hierarchy of multi-model approaches provides a promising way to better quantify uncertainties and decipher the relative contribution from internal dynamics and external forcings embedded in proxy records, particularly regarding ENSO.

How to cite: Gaudin, A. and Khodri, M.: New classes of climate model emulators to improve paleoclimate reconstructions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19188, https://doi.org/10.5194/egusphere-egu26-19188, 2026.

EGU26-19829 | Posters on site | NP3.3

Extending the Fresnel Platform with a 3D Isometric Graphical Interface for Land-Use Scenario Design in Hydrological Modeling   

Guillaume Drouen, Daniel Schertzer, Auguste Gires, Pierre-Antoine Versini, and Ioulia Tchiguirinskaia

Urban areas are increasingly exposed to localized extreme rainfall events, with evidence suggesting a trend toward higher precipitation volumes and more frequent short-duration, high-intensity storms, posing major challenges to infrastructure resilience and public safety. 

Urban hydrometeorology is characterized by highly nonlinear processes, strong interactions with geophysical systems, and pronounced variability across spatial and temporal scales, making both scientific understanding and operational management particularly demanding. 

Within this context, the Fresnel platform is a state-of-the-art urban hydrometeorological observatory combining conceptual modeling approaches with extensive field measurements. One of its components, RadX, is a Software-as-a-Service (SaaS) platform that provides real-time and historical data from high-resolution sensors, together with a graphical user interface (GUI) for Multi-Hydro, a fully distributed and physically based hydrological model developed at École nationale des ponts et chaussées (ENPC). Multi-Hydro relies on four open-source software components representing different processes of the urban water cycle. The RadX GUI allows users to efficiently run simulations using dedicated high-performance computing resources, configure multiple scenarios for a given catchment, modify land-use parameters, and assess their impacts on drainage system discharges. 

The originality of this contribution lies in the development of a new 3D isometric graphical interface based on an open-source game engine. Unlike conventional interfaces relying on the editing of raster matrices, this approach provides a more intuitive and spatially explicit visualization of land-use configurations. It enables a clearer representation and manipulation of Nature-based Solutions (NbS), such as porous pavements, whose implementation often remains abstract when expressed solely through raster data. 

Beyond hydrological modeling, RadX also supports integrating shared value principles into business models to enhance resilience and sustainability. Within the PIA3 TIGA-CFHF project (“Construire au futur, habiter le futur”), it promotes an integrated vision where economic activities are situated within a complex socio-environmental system, aligning economic performance with environmental and societal objectives. 

To support this transition, RadX aims to incorporates multifractal and advanced socio-economic analysis tools that enable organizations to assess performance and develop shared value–oriented strategies aligned with measurable environmental objectives. 

The RadX platform is continuously improved through an iterative development process driven by feedback from students, academic researchers, and industry practitioners, and may integrate additional visualization or forecasting components in future developments. 

How to cite: Drouen, G., Schertzer, D., Gires, A., Versini, P.-A., and Tchiguirinskaia, I.: Extending the Fresnel Platform with a 3D Isometric Graphical Interface for Land-Use Scenario Design in Hydrological Modeling  , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19829, https://doi.org/10.5194/egusphere-egu26-19829, 2026.

EGU26-20114 | Orals | NP3.3

Geophysical extremes, scaling and fractal support induced by zero-values 

Ioulia Tchiguirinskaia, Auguste Gires, and Daniel Schertzer

In the era of the data-driven research, the zero-values of geophysical fields require increased attention in order to improve understanding of their effective impacts on the prediction of extreme geophysical phenomena.

In everyday life, we use the idea that zero denotes the absence of quantity, whereas in geophysics, it refers to a chosen reference point, not necessarily the absence of a physical phenomenon.  It then results from the removal of the background field, either by design of the measured quantity or due to the current limitations of empirical detection.

Regardless of their origin, the presence of zeros in data significantly alters the resulting statistical distributions and influences the estimates of statistical parameter. Regarding universal multifractals (UM), two approaches have been favoured over the last thirty years to mimic the appearance of zeros and/or quantify their influence on the resulting UM estimates. The first, among the most widely used, relies on multiplying of a UM field by an independent fractal model, the ‘beta-model’, i.e. to assume the field has physically a fractal support. The second consist of thresholding the UM singularities and ignoring the fluctuations below the threshold, i.e. assuming that there is a detection of low field values.

This presentation will revisit these two approaches, emphasizing the significant resulting differences in the theoretical behaviour of the multifractal phase transitions, which are responsible for the behaviour of multifractal extremes. Then practical methods for preliminary detection of the most appropriate zero-creation mechanism within the data will be illustrated with concrete examples from geophysical fields.

How to cite: Tchiguirinskaia, I., Gires, A., and Schertzer, D.: Geophysical extremes, scaling and fractal support induced by zero-values, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20114, https://doi.org/10.5194/egusphere-egu26-20114, 2026.

EGU26-20699 | ECS | Orals | NP3.3

Multifractal Analysis of the Large-Scale Galaxy Distribution 

Dariusz Wójcik and Wiesław M. Macek

This study examines the large-scale structure of the visible universe to determine if fractal scaling laws offer a plausible explanation for the distribution of galaxies. Using the extensive Updated CfA Redshift (Z) CATalog (UZCAT) compilation, which includes redshift data for around one million galaxies, we identify a reliable multifractal spectrum of the galaxy distribution on cosmological scales.

By calculating the generalized dimensions Dq and the singularity spectrum f (α), we demonstrate that the observed distribution is consistent with the weighted Cantor set model, indicative of nonlinear multifractal scaling. We find that the one-scale model parameter (p ≈ 0.45) relates to the presence of voids in the large-scale distribution of matter. Furthermore, the observed asymmetry in the spectrum may be explained by variations from the Hubble law for ideal uniform expansion

Interestingly, the overall shape of the multifractal spectrum resembles that observed by NASA's Voyager missions at the heliospheric boundaries, suggesting some universal properties of scaling across these different physical systems. However, the degree of multifractality for galaxies (Δ ≈ 0.1 – 0.17) is notably smaller than that found in heliospheric turbulence, indicating distinct underlying physical constraints despite the shared mathematical methodology.

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 and D. Wójcik, 2026, Fractal Nature of Galaxy Clustering in the Updated CfA Redshift Catalog, Sci. Rep., https://doi.org/10.1038/s41598-026-36013-3.

[2] W. M. Macek, A. Wawrzaszek, and L. F. Burlaga, 2014, Multifractal structures detected by Voyager 1 at the heliospheric boundaries.
Astrophys. J. Lett. 793, L30. https://doi.org/10.1088/2041-8205/793/2/L30.

How to cite: Wójcik, D. and Macek, W. M.: Multifractal Analysis of the Large-Scale Galaxy Distribution, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20699, https://doi.org/10.5194/egusphere-egu26-20699, 2026.

EGU26-21023 | ECS | Posters on site | NP3.3

A Dye-Tracer Forward-Modeling Framework for Deglacial Meltwater Reconstruction 

Laura Endres, Ruza Ivanovic, Yvan Romé, and Heather Stoll

Freshwater input from melting polar ice sheets can profoundly alter ocean circulation, in particular the Atlantic Meridional Overturning Circulation (AMOC), with far-reaching climatic consequences. Yet the sensitivity of the AMOC to freshwater forcing remains highly uncertain: models exhibit divergent responses depending on source location, background climate state, and circulation regime, while the instrumental record is too short to unambiguously detect and characterise a melt-driven weakening.

Palaeoclimate archives, especially from the last deglaciation, provide ample evidence of melt events through indicators such as surface-ocean δ¹⁸O and biomarkers (e.g. BIX) in sediment cores and speleothems. However, the spatial and temporal characteristics of the underlying meltwater forcing remain poorly constrained. While meltwater discharge into the North Atlantic may be local, rapid, and event-like, its redistribution and impact on the AMOC unfold over centuries, complicating direct inference from surface-ocean proxies. Consequently, in deglacial general circulation model simulations, meltwater forcing is typically inferred indirectly from ice-sheet reconstructions or expected climate responses, resulting in a wide spread of applied forcings that propagates into substantial uncertainty.

Here we introduce a new forward-modelling approach aimed at strengthening the estimation and detection of regionally distinct and temporally evolving surface-ocean meltwater signals in proxy archives. We develop an empirical Green’s-function (impulse-response) framework based on a new suite of HadCM3 simulations, in which conservative tracers track meltwater originating from different source regions under distinct AMOC modes representative of deglacial conditions. Signals at terrestrial proxy sites are inferred using atmospheric back-trajectory analysis. The resulting kernels encode the system’s response for different source regions across multiple time lags, allowing any transient meltwater history to be reconstructed through discrete convolution with a derived 500-year response function. Applied to the last deglaciation, the framework demonstrates how differences between ice-sheet reconstructions (e.g. GLAC-1D versus ICE-6G) translate into distinct surface-ocean meltwater anomalies in the North Atlantic. The model highlights the critical role of meltwater amount, timing, and injection location, as well as the underlying AMOC circulation mode, in shaping surface-ocean proxy signals. It further provides quantitative estimates of how meltwater-related surface anomalies propagate to proxy sites distributed across the North Atlantic. Notably, transitions between AMOC modes can effectively mask even massive meltwater pulses, such as Meltwater Pulse 1A, at certain proxy locations. This forward-modelling approach thus offers an alternative perspective on deglacial freshwater forcing in the proxy realm and represents a step towards data-constrained reconstructions of past surface-ocean freshening and AMOC resilience.

How to cite: Endres, L., Ivanovic, R., Romé, Y., and Stoll, H.: A Dye-Tracer Forward-Modeling Framework for Deglacial Meltwater Reconstruction, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21023, https://doi.org/10.5194/egusphere-egu26-21023, 2026.

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

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

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

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

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

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

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

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

EGU26-10741 | ECS | Orals | GI2.4

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

siddaling Bakka and Sudardeva Narayanan

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

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

EGU26-11280 | Orals | GI2.4

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

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

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

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

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

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

EGU26-12001 | Orals | GI2.4

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

Ankit Balvanshi, Jayakumar Kv, and Venkappayya r Desai

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

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

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

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

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

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

EGU26-12042 | ECS | Posters on site | GI2.4

Strategies for spatial leave-one-out cross-validation 

Cristina Olimpia Chavez Chong, Cécile Hardouin, and Ana Karina Fermin Rodriguez

The purpose of the talk is to discuss spatially adapted cross-validation methods that maintain sufficient separation between training and validation sets, thus providing more accurate estimates of model risk. We begin by reviewing various spatial cross-validation techniques, including spatial blocked cross-validation and spatial leave-one-out, under scenarios of low to strong spatial dependence. We then propose a practical framework for determining an optimal “buffer size” for spatial leave-one-out that reduces autocorrelation between training and validation subsets. This framework is further enhanced by a parametric bootstrap approach designed to approximate the true risk in single-realization settings. Simulation experiments confirm that these methods effectively capture the underlying spatial structure, leading to more reliable risk estimation.

How to cite: Chavez Chong, C. O., Hardouin, C., and Fermin Rodriguez, A. K.: Strategies for spatial leave-one-out cross-validation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12042, https://doi.org/10.5194/egusphere-egu26-12042, 2026.

EGU26-13261 | ECS | Orals | GI2.4

Flow Modulation and Wave Impact Reduction by Retreated Crown Walls in Vertical Breakwaters 

Shaik Firoj and Mohammad Saud Afzal

This study investigates wave-induced flow behaviour around vertical breakwaters with retreated crown wall using numerical simulations. Previous experimental work has shown that moving the crown wall landward can reduce wave forces, moments, and overtopping. However, the associated flow mechanisms near the wall and trunk region have not been examined in detail. In this work, the open-source CFD model REEF3D is used to simulate regular wave interaction for crown wall retreat configuration. The model solves the Reynolds-averaged Navier–Stokes equations, with a level set method for free-surface tracking and a k–ω turbulence closure. The numerical results are first validated against published experimental data to ensure accuracy. The simulations provide detailed information on velocity fields, vortex formation, and flow separation during wave impact and overtopping. The results show that retreating the crown wall modifies the local flow structure, leading to a redistribution of momentum and a reduction in direct wave impact on the wall. These findings help to clarify the hydrodynamic role of retreated crown wall in vertical breakwater design.

How to cite: Firoj, S. and Afzal, M. S.: Flow Modulation and Wave Impact Reduction by Retreated Crown Walls in Vertical Breakwaters, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13261, https://doi.org/10.5194/egusphere-egu26-13261, 2026.

Watershed hydrodynamics is governed by various hydrological flow processes that occur at different spatiotemporal scales. Most hydrological models couple the surface flow solver with the standard empirical infiltration models for flood propagation modeling. However, the empirical infiltration models are not applicable for heterogeneous and anisotropic soils and shallow groundwater tables, which are most vulnerable to waterlogging problems. Hence, simultaneous and integrated modeling of the surface and subsurface flow processes is essential for the continuous monitoring of watershed hydrodynamics. A physically based unified multi-region, multi-process watershed model integrates the various hydrological flow components in different regions through unique coupling mechanisms at the interfaces. The current work presents a Finite Volume (FV) method-based watershed flow model developed using the OpenFOAM® framework [1]. The developed model framework utilizes the ‘multi-region’ structure from the OpenFOAM® library to integrate the OpenFOAM®-based solvers for the individual processes of surface overland flow [2,3] and saturated-unsaturated subsurface flow [4] through the imposition of appropriate interface boundary conditions or addition of source/sink terms at the interfaces of the flow regions. The surface flow component is modeled using the diffusive wave or the zero-inertia (ZI) approximation of the two-dimensional (2D) depth-averaged shallow water equations (SWE). On the other hand, the flow through the variably saturated subsurface media is modeled using the ‘mixed form’ of the 3D modified Richards Equation. The flux exchange between the surface and subsurface regions (infiltration or exfiltration rate) is modeled using a switching algorithm to impose the boundary condition on the interface between the two regions. The algorithm changes the interface to a Dirichlet or a Neumann type boundary condition based on the rainfall intensity and the saturated hydraulic conductivity of the ground surface. A stabilized and adaptive time-stepping algorithm has been implemented to ensure smooth convergence of the iterative technique used for linearizing the nonlinear governing equations. The developed model is equipped with parallelization strategies to be run on multi-core processors, which is essential for increased computational efficiency while solving regional-scale watershed flow problems. The developed watershed model has been verified and validated against the standard benchmark problems on saturation excess and infiltration excess from the literature. Moreover, the applicability of the developed model has been extended to solve complex hydrological problems on exfiltration occurring over natural catchments, yielding satisfactory results.

References

[1] Jasak, H., A. Jemcov, Z. Tukovic. (2007). OpenFOAM: A C++ library for complex physics simulations. In Vol. 1000 of Proc., Int. Workshop on Coupled Methods in Numerical Dynamics,1–20. Dubrovnik, Croatia: Inter-University Center

[2] Dey, S., Dhar, A. (2024). Applicability of Zero-Inertia Approximation for Overland Flow Using a Generalized Mass-Conservative Implicit Finite Volume Framework. Journal of Hydrologic Engineering, 29(1), 04023042.

[3] Dey, S. (2025). zeroInertiaFlowFOAM – a OpenFOAM®-based computationally efficient, mass-conservative, implicit zero-inertia flow model for flood inundation problems on collocated grid-systems (No. EGU25-17402). Copernicus Meetings.

[4] Dey, S., & Dhar, A. (2022). Generalized mass-conservative finite volume framework for unified saturated–unsaturated subsurface flow. Journal of Hydrology, 605, 127309.

How to cite: Dey, S. and Dhar, A.: An OpenFOAM®-based coupled surface-subsurface flow model for simulating watershed hydrodynamics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13540, https://doi.org/10.5194/egusphere-egu26-13540, 2026.

EGU26-16374 | ECS | Orals | GI2.4 | Highlight

Reorganization of Heatwave Day Regimes across India under Recent and Near Future Warming 

Srikanth Bhoopathi and Manali Pal

Heatwaves are among the most rapidly intensifying climate extremes over India, yet their evolving spatial characteristics under recent and near future climate change remain inadequately quantified. This study examines the spatio-temporal variability of Heatwave Days (HWDs) across India using daily maximum temperature from the India Meteorological Department (IMD) gridded dataset for the historical period 1975-2024 and extends the analysis to the near future (2025-2044) using CMIP6 climate projections. Heatwave days are identified at each grid point using a calendar day based percentile approach, where daily maximum temperature exceeding the local 95th percentile threshold for the same calendar day, computed over a fixed reference period of 1981-2010, is classified as a heatwave day. Grid wise cumulative and decadal HWDs are analysed to assess long-term exposure and spatial redistribution. To objectively identify dominant heatwave regimes, Self-Organizing Maps (SOMs) are employed using multiple HWD metrics, enabling classification of regions with distinct heatwave characteristics and temporal evolution. Observational results indicate a clear reorganization of heatwave patterns over India. During the late 20th century (1975-1994), HWD accumulation is largely limited to north-western and parts of central India, typically ranging between 26 to 50 days per decade, with most eastern and peninsular regions experiencing fewer than 25 HWDs. From the mid-1990s onward, a pronounced intensification and spatial expansion is evident. By 2005-2014, large parts of central and eastern India exhibit decadal HWDs in the range of 51 to 100 days. The most recent decade (2015-2024) shows widespread moderate to high HWDs accumulation across the country, with several regions of central, eastern, and peninsular India experiencing 101 to 150 HWDs, and localized hotspots exceeding 150 days per decade. Future HWDs for 2025-2044 are derived from daily maximum temperature projections of the MPI-ESM1-2-HR model under the SSP2-4.5 scenario. The near-future decadal projections (2025-2034 and 2035-2044) indicate a continued intensification and spatial expansion of HWDs, with extensive areas of north-western, central, and peninsular India experiencing 151 to 250 HWDs per decade, and emerging hotspots exceeding 250 to 350 days, particularly over parts of north-western and southern India. Eastern India also shows a marked transition toward higher HWDs classes, indicating increasing regional vulnerability. Overall, the combined observational and CMIP6 based analysis demonstrates a transition toward widespread and persistent heatwave exposure across India in both recent decades and the near future. The integration of a grid specific, calendar day based percentile definition with SOM based classification provides a robust framework for identifying evolving heatwave regimes and supports improved heat risk assessment, climate adaptation planning, and early warning strategies under continued warming.

How to cite: Bhoopathi, S. and Pal, M.: Reorganization of Heatwave Day Regimes across India under Recent and Near Future Warming, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16374, https://doi.org/10.5194/egusphere-egu26-16374, 2026.

Considering the dearth of gauge-based rainfall observations at desirable resolution, it becomes immensely challenging to quantify and monitor droughts, especially over the developing countries. This can be circumvented by utilizing the high-resolution open-access rainfall products. This study is envisaged with the objective to assess the spatiotemporal variation of meteorological droughts over the Bundelkhand region, India. The multi-source weighted-ensemble precipitation (MSWEP), a blended product of global gauge-based, satellite-based and reanalysis precipitation datasets, is utilized for a period of 44 years (1980-2023). The MSWEP rainfall is bias-corrected with respect to the India Meteorological Department (IMD) gridded observation dataset for the 14 districts in the region. Using the corrected rainfall product, the droughts over each district are characterized by Standardized Precipitation Index (SPI) at three different timescales, i.e., the SPI-3, SPI-6 and SPI-12 are used to model short-term, intermediate-term and long-term droughts, respectively. A drought severity index (DSI) is proposed considering the probability of droughts in different severity classes (i.e., near-normal, moderate, severe and extreme). Further, the trend analysis of SPI at different timescales is carried out using Modified Mann-Kendall (MMK) test. The results reveal the MSWEP dataset’s problems in capturing higher quantiles, which affects the probabilistic distribution used for quantifying drought events. However, the bias-corrected MSWEP product showed an excellent match with the IMD gridded data, thereby substantiating its applicability over the Bundelkhand Region. The region is found to be prone to droughts with an increasing trend of dryness. The novel approach of DSI is found to distinguish the drought severity levels at district-scale, which can be helpful for planning and management of droughts. Overall, this study provides critical insights on the drought characterization using state-of-the-art datasets and innovative approaches, which can also be extended to other drought-prone regions of the world.

 

Keywords: Bias-correction; Bundelkhand; DSI; MSWEP; MMK; SPI

How to cite: Swain, Dr. S.: A statistical approach of mapping drought severity using bias-corrected blended dataset over a semi-arid region, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18814, https://doi.org/10.5194/egusphere-egu26-18814, 2026.

EGU26-18906 | Orals | GI2.4

Passive Acoustic Characterization of Marine Bedload Transport Based on Interparticle Collision Dynamics 

Debasish Dutta, Armelle Jarno, Hugues Besnard, Bruno Morvan, and Francois Marin

Marine sediments are very important for keeping the coast stable and protecting the shoreline naturally. However, anthropogenic activities can greatly change how sediment moves, making their accurate monitoring essential. In marine settings, understanding bedload sediment transport can be challenging due to conventional methods reliant on visual observations or direct sediment sampling tend to be intrusive, spatially constrained, and inadequate for long-term or continuous monitoring. In this situation, passive underwater acoustics is a promising non-intrusive option that can provide continuous monitoring with high temporal resolution. This study investigates the acoustic signatures related to marine bedload transport, focusing particularly on the sounds generated by interparticle collisions of mobile sediments. A series of controlled laboratory experiments are performed utilising simplified experimental arrangements in which artificial sediments (spherical glass beads) are mobilised under oscillatory motion that simulates wave-induced seabed forcing. We use glass beads of different sizes to create idealised bedload conditions, and we use an oscillating plate to control the movement of the particles. Hydrophones placed close to the sediment bed record acoustic pressure signals. The recorded acoustic signals are analyzed in both the time and frequency domains. Individual particle impacts are characterised by short transient acoustic events, and spectral analyses show clear peak frequencies that are linked to sediment motion. The results indicate that the peak frequency of the acoustic spectrum is predominantly determined by particle diameter and is additionally influenced by the amplitude and frequency of the applied oscillatory motion. These observations align with theoretical models, such as those suggested by Thorne (1985), that explain the generation of pressure waves during underwater particle collisions. To further explore the mechanisms of sound generation, experiments are conducted with both smooth and rough beds below the beads layers. The analysis reveals the existence of sediment-specific acoustic signatures, facilitating the differentiation of particle sizes according to their spectral characteristics. This study illustrates the significant potential of passive acoustic methods for the remote monitoring of marine bedload transport. The study offers novel insights into sound generation mechanisms linked to sediment motion across various particle sizes, motion amplitudes, and bed configurations, utilising a combination of laboratory experiments, theoretical frameworks, and comprehensive spectral analysis, with direct implications for intricate coastal and offshore environments.

How to cite: Dutta, D., Jarno, A., Besnard, H., Morvan, B., and Marin, F.: Passive Acoustic Characterization of Marine Bedload Transport Based on Interparticle Collision Dynamics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18906, https://doi.org/10.5194/egusphere-egu26-18906, 2026.

To investigate the microphysical characteristics of summer precipitation in the Northern Yellow River Irrigation Area, the Central Arid Zone, and the Southern Mountainous Area of Ningxia, this study analyzed disdrometer data collected from Yinchuan, Yanchi, and Liupanshan stations from 2022 to 2024. A comparative analysis of Raindrop Size Distribution (RSD) was conducted from the perspectives of the overall dataset, different rainfall rates, and precipitation types. The results indicate that the average RSD at Liupanshan station is broader with a higher number concentration of small raindrops, whereas the average RSD at Yinchuan station is narrower with a higher concentration of mid-size raindrops. Under different rainfall rates and precipitation types, the number concentrations of both small and large raindrops increase with rising altitude. Specifically, when the rainfall rate is less than 2mm·h-1, the mass-weighted mean diameter (Dm) gradually decreases while the normalized intercept parameter (log10NW) increases with altitude. When the rainfall rate exceeds , the log10NW at Yanchi and Liupanshan stations surpasses that of Yinchuan station, whereas the Dm is smaller than that of Yinchuan. Furthermore, for a given shape parameter (µ), the slope parameter (⋀) increases with altitude. In convective precipitation events, the empirical relationships tend to overestimate the rainfall intensity at all three stations when the rainfall rate exceeds 20mm·h-1.

How to cite: Xue, Z.: Characteristics of Raindrop Spectrum in different areas of Ningxia during Summer, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2128, https://doi.org/10.5194/egusphere-egu26-2128, 2026.

EGU26-5139 | ECS | PICO | HS7.1

Adaptive K–R relationships based on cloud phase classification using SEVIRI observations 

Taoufiq Shit, Martin Fencl, and Vojtěch Bareš

Errors in the representation of the drop size distribution are a major source of uncertainty in rainfall estimation, since both radar reflectivity and microwave attenuation depend nonlinearly on precipitation microphysics. These uncertainties propagate directly into the specific attenuation–rain rate (k–R) relationship through the interaction between electromagnetic waves and hydrometeors, leading to systematic biases when globally fixed coefficients are used. In standard practice, the k–R relationship is expressed as a power law of the form k=aRb, where the coefficients a and b are typically taken from the International Telecommunication Union (ITU) recommendations and assumed to be globally applicable. The use of the ITU coefficients implicitly assumes stationary rainfall microphysics, which is physically inconsistent under varying cloud and rain regimes. This highlights the need for stratified parameterizations in which the coefficients are optimized for different microphysical conditions. In this context, cloud phase information from geostationary satellites provides a physically meaningful basis for clustering the k–R relationship, as different cloud phases are associated with distinct precipitation formation processes and drop size distributions.

The objective of this study is to derive cloud phase dependent k–R parameterizations and to assess their performance across a large disdrometer network. A global disdrometer dataset (Ghiggi et al., 2021, DISDRODB) covering multiple climatic regions is used to simulate k–R relationships across a wide frequency range from 5 to 100 GHz using the T-matrix scattering method. SEVIRI MSG observations are used as input to the Cloud Physical Properties (CPP) product provided by the EUMETSAT Climate Monitoring Satellite Application Facility (CM SAF), from which cloud phase is classified into water, supercooled water, mixed phase, deep convective, cirrus, and opaque ice categories. Frequency dependent k–R coefficients are derived separately for each cloud type. The framework is evaluated across more than 100 independent disdrometer sites, primarily concentrated in Europe.

Relative to the ITU recommended model (ITU-R P.838-3), the cloud phase adaptive parameterization substantially reduces root mean square error (RMSE), with the strongest improvements observed at 5 to 8 GHz. At these frequencies, more than 90 percent of sites show lower RMSE, with average reductions reaching up to 1.5 mm.h-1. More moderate improvements are found at higher frequencies from 60 to 100 GHz, where around 60 percent of sites show RMSE reductions, with average improvements below 0.5 mm.h-1.

These results show that cloud phase informed k–R parameterizations can significantly improve rainfall estimation from commercial microwave links and indicate potential applicability to radar systems.

Reference:

Ghiggi, G., Billault-Roux, A. C., Candolfi, K., Pillac-Mage, L., Unal, C., Schleiss, M., Uijlenhoet, R., Raupach, T., and Berne, A.: DISDRODB – A global disdrometer archive of raindrop size distribution observations, PrePEP 2025, Karlsruhe, Germany, 10–12 March 2025, https://indico.kit.edu/event/4015/contributions/18545/, 2025.

 

This work was supported by the Czech Science Foundation (GACR), Czech Republic, under Grant No. 24-13677L (MERGOSAT).

How to cite: Shit, T., Fencl, M., and Bareš, V.: Adaptive K–R relationships based on cloud phase classification using SEVIRI observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5139, https://doi.org/10.5194/egusphere-egu26-5139, 2026.

EGU26-6612 | ECS | PICO | HS7.1

Do Satellite-Based Precipitation Datasets Capture Flash Flood-Producing Cloudburst Events? 

Nandana Dilip K and Vimal Mishra

Cloudbursts and mini-cloudbursts are on the rise over India, frequently triggering flash floods. According to the India Meteorological Department (IMD), a cloudburst is defined as rainfall exceeding 100 mm in an hour over a spatial extent of 20-30 km², while mini-cloudbursts are characterized by rainfall of about 50 mm in an hour. Although IMD issues cloudburst reports within 24 hours of occurrence, accurate identification and categorization of these events remain challenging in several regions due to the sparse distribution of meteorological stations, particularly in complex terrain. Satellite-based observations provide high spatial coverage and can detect intense clouding or heavy rainfall events. However, satellites often infer rainfall or cloud properties from radiance, which can introduce uncertainties compared to direct ground measurements. Here, we assess how effectively satellite-based precipitation datasets capture cloudburst events over India by comparing satellite-based rainfall estimates with station-based hourly observations. We evaluate the performance of IMERG and ERA5-Land datasets to identify regions where satellites successfully detect cloudburst events and regions where their performance is limited across India. The results aim to improve understanding of the regional strengths and limitations of satellite datasets for monitoring extreme rainfall and enhancing flash flood preparedness in data-sparse regions of India.

How to cite: Dilip K, N. and Mishra, V.: Do Satellite-Based Precipitation Datasets Capture Flash Flood-Producing Cloudburst Events?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6612, https://doi.org/10.5194/egusphere-egu26-6612, 2026.

Precipitation falling onto vegetation is partly intercepted by the canopy and subsequently evaporates, while the remainder reaches the ground as throughfall or stemflow. Throughfall refers to precipitation that reaches the ground after crossing the canopy. It comprises free throughfall (raindrops not intercepted), drips, and splash droplets. Different rainfalls and foliage yield different number, size and velocity of each throughfall droplet type [1]. The resulting drop size distribution significantly affects infiltration and surface runoff processes [2]. Moreover, drips may induce the erosion and compaction of bare soil [3] while splash droplets may transport pathogenic spores [4]. Finally, the part of leaves that remains wet may experience significant leaching or water/nutrient uptake [5].

Predicting throughfall drop size distribution with physical models is complex because the physically relevant scale is that of a raindrop impacting a leaf, while the scale of interest is at least that of a tree. Previous studies (e.g., [6-8]) provided measurements at either scale but never at both. A few numerical models [4, 9-10] were proposed to estimate throughfall statistics and rain-induced transport by modelling interception at raindrop scale, but these models relied on strong and unverified assumptions on drop-scale dynamics.

In this original study, we first provide a detailed experimental characterization of interception at leaf scale. Hundreds of raindrop surrogates impacted single birch leaves. The leaf was weighed and imaged over time, and water storage variations were resolved at the scale of individual impacts. The storage capacity, the wetting-up time, the drip diameter and the splash fraction were measured as functions of the leaf area, the leaf inclination and the raindrop size. The results are extensively compared to previous studies at leaf scale.

Then rain interception is quantified at tree scale, with the same birch species and leaves in the same phenophase. Rain amount, intensity and drop size distribution in both open rainfall and throughfall were measured using two disdrometers positioned respectively above and below the canopy of a birch tree. Free throughfall, splash droplets and drips were separated for selected rainfall events with different intensities. The storage capacity and the wetting-up time were also estimated for each event. We relate these tree-scale measurements to the mechanisms observed at the leaf scale.

[1] D. F. Levia et al., Hydrol. Process. 33, 1698-1708 (2019)

[2] K. Nanko et al., Hydrol. Process. 24, 567-575 (2010)

[3] M. Beczek et al., Geoderma 347, 40-48 (2019)

[4] T. Vidal et al., Ann. Bot. 121, 1299-1308 (2018)

[5] T. E. Dawson and G. R. Goldsmith, New Phytol. 219, 1156-1169 (2018)

[6] C. Bassette and F. Bussière, Agric. For. Meteorol. 148, 991-1004 (2008)

[7] X. Li et al., Agric. For. Meteorol. 218, 65-73 (2016)

[8] C. D. Holder, Ecohydrol. 6(3), 483-490 (2012)

[9] Q. Xiao et al., J. Geophys. Res. 105 (D23), 29173-29188 (2000)

[10] R. P. de Moraes Frasson and W. F. Krajewski, J. Hydrol. 489, 246-255 (2013)

How to cite: Gilet, T. and Zabret, K.: Bridging the scales of rainfall interception, from raindrop impacts on leaves to throughfall under a tree., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6681, https://doi.org/10.5194/egusphere-egu26-6681, 2026.

Accurate rainfall measurement remains challenging, even for in-situ point observations commonly considered the “ground truth”, owing to precipitation undercatch primarily caused by wind effects and instrument design. These biases limit reliable rainfall estimation, especially at very high and low intensities, and hinder the robust characterisation of precipitation variability. This study first used disdrometer data from multiple sites across the UK to develop a new rainfall classification system based on observed drop size distributions rather than intensity thresholds alone. The proposed classification distinguished periods of rainfall with similar bulk intensities but different microphysical structures, providing a more physically meaningful framework for precipitation characterisation and supporting the development of more targeted undercatch correction strategies. Second, a custom-built rainfall simulator was developed to replicate the identified rainfall types under controlled laboratory conditions. The simulator enables independent control of rainfall rate and drop size distribution, allowing the reproduction of a wide range of precipitation regimes representative of natural UK rainfall. Controlled experiments were used to systematically quantify the response of rain gauges to different drop populations and intensities, providing new insights into the mechanisms driving undercatch and its dependence on rainfall microstructure. By explicitly linking drop-scale processes, controlled experimentation, and population-level rainfall classification, this work contributes to the improved accuracy of precipitation measurements and the representation of rainfall at hydrologically relevant scales, with direct implications for rainfall monitoring, model input uncertainty, and flood risk assessment.

How to cite: Dunn, R., Fowler, H., Green, A., and Lewis, E.:  Understanding Rain Gauge Undercatch Through Drop Size Distribution–Based Rainfall Classification and Artificial Rainfall Generation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7894, https://doi.org/10.5194/egusphere-egu26-7894, 2026.

EGU26-10315 | PICO | HS7.1

Leveraging opportunistic rainfall sensors to improve hydrological flood modelling in a peri-urban catchment 

Andrijana Todorović, Nebuloni Roberto, De Michele Carlo, Cazzaniga Greta, Deidda Cristina, Kovačević Ranka, and Ceppi Alessandro

Accurate flood simulations necessitate rainfall inputs with fine spatiotemporal resolution, especially if semi- or fully-distributed hydrological models are used. Rainfall data are commonly obtained from rain gauges and/or weather radars, each with their associated uncertainties and challenges, especially with capturing heavy, localised events, and with high implementation- and maintenance costs [1]. This further translates into high costs of hydrological modelling of flood events [2].

An interesting alternative to rain gauges and radars are the rainfall data gathered from opportunistic sensors, such as Commercial Microwave Links (CMLs). CML data come at no infrastructure cost as they are generated by the network management system of mobile networks to monitor link performance. Furthermore, CMLs cover a large part of the world. Their strong potential to providing near-surface, fine-resolution rainfall fields has been demonstrated in many studies [3]. However, their usage for hydrological modelling has been little investigated so far. CML data have been mostly used for fully-distributed models in small catchments with an area of few square kilometres [1], with isolated examples of application in large catchments and/or with semi-distributed models [1],[4].

In this study, we analyse the impact of various modelling decisions about application of CML rainfall data on simulated flood hydrographs. Specifically, selection of (i) the approach to pre-processing CML signals to obtain hyetographs [3], (ii) CML data usage as a standalone input or in a combination with conventional datasets, and (iii) the way to calculate sub-catchment-averaged rainfall, are analysed. Different rainfall inputs are created accordingly, and used to force a semi-distributed model of the pre-alpine, peri-urban Lambro catchment in northern Italy notorious for intensive, tightly-localised events that trigger floods [4]. The simulated hydrographs of twelve flood events are compared to the observed ones in terms of the Nash-Sutcliffe coefficient, relative errors in peak magnitudes and runoff volumes, and timing of peak occurrence. Based on our analyses, specific recommendations are provided, with the ultimate goal to promote a wider application of CML data for hydrological modelling.

 

Acknowledgments

The authors would like to thank the “OpenSense” COST Action (CA20136) for supporting their collaboration through the STSM program.

References

[1]           J. Olsson et al., ‘How close are opportunistic rainfall observations to providing societal benefit?’, Journal of Hydrometeorology, Aug. 2025, doi: 10.1175/JHM-D-25-0043.1.

[2]           J. Seibert, F. M. Clerc‐Schwarzenbach, and H. J. (Ilja) Van Meerveld, ‘Getting your money’s worth: Testing the value of data for hydrological model calibration’, Hydrological Processes, vol. 38, no. 2, p. e15094, Feb. 2024, doi: 10.1002/hyp.15094.

[3]           S. C. Doshi, C. De Michele, G. Cazzaniga, and R. Nebuloni, ‘A Framework for Minimizing the Impact of Wet Antenna Attenuation on Rainfall Estimates Provided by Commercial Microwave Links’, IEEE J. Sel. Top. Appl. Earth Observations Remote Sensing, vol. 19, pp. 421–437, 2026, doi: 10.1109/JSTARS.2025.3632933.

[4]           G. Cazzaniga, C. De Michele, M. D’Amico, C. Deidda, A. Ghezzi, and R. Nebuloni, ‘Hydrological response of a peri-urban catchment exploiting conventional and unconventional rainfall observations: the case study of Lambro Catchment’, Hydrol. Earth Syst. Sci., vol. 26, no. 8, pp. 2093–2111, Apr. 2022, doi: 10.5194/hess-26-2093-2022.

How to cite: Todorović, A., Roberto, N., Carlo, D. M., Greta, C., Cristina, D., Ranka, K., and Alessandro, C.: Leveraging opportunistic rainfall sensors to improve hydrological flood modelling in a peri-urban catchment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10315, https://doi.org/10.5194/egusphere-egu26-10315, 2026.

Rainfall retrieval algorithms for weather radars are linked to assumptions about drop size distributions (DSDs), but DSD properties vary strongly across rainfall regimes. To reduce regime-dependent biases in radar-based quantitative rainfall estimation, we use high-temporal-resolution disdrometer observations to quantify microphysical differences between strong convection, embedded convection, and stratiform rainfall with a bright-band, and to test how well these regimes can be separated in the (Dm, log10Nw) phase space, where Dm is the mass-weighted mean diameter and Nw the normalized intercept parameter.

Our analysis shows a systematic convective–stratiform contrast. Strong convection has larger characteristic drop sizes and higher normalized concentrations (mean Dm ≈ 1.07 mm; mean Nw ≈ 2.93 × 104 m−3 mm−1). Embedded convection has slightly smaller Dm but Nw remains comparably high (mean Dm ≈ 1.02 mm; mean Nw ≈ 2.00 × 104 m−3 mm−1). Stratiform rainfall with a bright-band has smaller Dm and markedly lower Nw (mean Dm ≈ 0.92 mm; mean Nw ≈ 6.38 × 103 m−3 mm−1).

Cumulative DSD curves indicate that regime separation is driven primarily by the large-drop tail: strong convection shows the highest contribution of drops above ~2–3 mm, embedded convection is intermediate, and stratiform rainfall declines steeply at large diameters. To translate these findings into an objective regime indicator, we train a linear SVM (Support Vector Machine) on canonical samples (strong convection vs stratiform rainfall with a bright-band) and apply it to all events. Convective and stratiform rainfall are largely separable, while embedded convection occurs on both sides of the boundary, supporting a probabilistic classification with a transition band. These results provide microphysical insights that can be used to refine regime-dependent radar retrieval parameterizations and improve radar-based rainfall estimates at hydrologically relevant scales.

How to cite: Rulfova, Z. and Potuznikova, K.: Disdrometer-based microphysical contrasts between convective and stratiform rainfall to improve radar rainfall retrievals, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10645, https://doi.org/10.5194/egusphere-egu26-10645, 2026.

Analyzing the transition probability of disdrometer data revealed a sigmoid relation between precipitation intensity of the current and next minute. The sigmoid changes in it's parameters slope, location and asymmetry based on the intensity of the current value. In particular the evolution of the parameters shows some distinct bends that mark transition points. Replicating how the sigmoid morphs with intensity we build a Markov chain model that generates realistic precipitation data. In particular it can generate the power law relation in the high intensity range of the distribution and also correctly includes a transition to exponential distribution at low intensities. To complete the algorithm we included a threshold based transition to dry periods. This introduces realistic intermittency into the data. What makes our findings compelling is that we strictly replicated the micro structures we found in the data and ended up with a random walk that generates the large scale structure of the data set. No optimizing was involved. We still have to fully validate the performance of our algorithm and understand the essential components that generate key characteristics as for example the transition between exponential and power law. With that we hope to find a universal mechanism that is able to generate very different precipitation distributions based on how we shape the morphing of the sigmoid function.

How to cite: Frechen, T. N. and Hinz, C.: Replicating the micro structure of disdrometer data leads to a rainfall generator that correctly reproduces the large scale structure of the data set, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11452, https://doi.org/10.5194/egusphere-egu26-11452, 2026.

EGU26-11781 | ECS | PICO | HS7.1

Multifractal analysis of Drop Size Distribution parameters vertical and temporal variability 

Emna Chikhaoui and Auguste Gires

Rainfall exhibits extreme spatial and temporal variability observable across wide range of scales. This variability is not limited to precipitation totals but also concerns the microphysical structure of the rain characterized with the help of the drop size distribution (DSD). It is defined as the number of raindrops per unit volume of air with a given equivolumic diameter. The  DSD can be described through its statistical parameters (basically its moments) such as the rain rate (RR), the liquid water content (LWC), the mass-weighted mean diameter (Dm) and the total number concentration (Nt). The vertical variability of DSD remains an active field of research, particularly due to the challenges associated with observing and generalizing microphysical profiles which are used to improve rainfall ground estimates from radar measurements.

Vertically-oriented radar measurements are a valuable tool for studying the vertical variability of DSD along the precipitation column with small spatial and short temporal observation scales. In this study, nine months of a Micro Rain Radar PRO (MRR-PRO) measurements were gathered in Ecole nationale des ponts et chaussées (ENPC), Institut Polytechnique de Paris (IPP), which is located in the eastern part of the Paris region, France. The MRR-PRO is a K-band weather radar that provides high-resolution vertical profiles of precipitation features that reach more than 4 kilometers of altitude above its position with a 35 meters spatial resolution and a 10 seconds time step. Based on the collected data and simple assumptions, several parameters related to the raindrop size distribution can be estimated empirically, such as RR, LWC, Dm and Nt. The spatial and temporal variability of the DSD was studied using the Universal Multifractal (UM) framework, a physically based framework designed to characterize geophysical fields across wide  range of scales through a limited set of physically interpretable parameters.

Two types of UM analysis were conducted in this study. First, the time series of DSD statistical moments is explored at each altitude. Then, vertical profiles of these moments are examined to extract UM parameters that characterize the variability along the vertical column. The results and their interpretation within a spatiotemporal framework will be presented.

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 Drop Size Distribution parameters vertical and temporal variability, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11781, https://doi.org/10.5194/egusphere-egu26-11781, 2026.

EGU26-12024 | ECS | PICO | HS7.1

Determination of Z-R Relationships for Rainfall Estimation from Weather Radar, Rain Gauges, and Disdrometers 

Nicolás Andrés Chaves González, Alessandro Ceppi, Carlo De Michele, Giovanni Ravazzani, and Orietta Cazzuli

Z-R relationships are a fundamental component of rainfall estimation and are widely applied in radar meteorology and hydrology supporting operational applications such as flood forecasting. Despite their extensive use, the procedures adopted to derive Z-R coefficients are often not described in sufficient detail, and key methodological choices, such as the selection of the dependent variable in the regression analyses, are frequently left implicit.

In this study, we analyze the determination of Z-R relationships using rain gauge, disdrometer, and X-band radar observations with solid-state transmitters collected over the Seveso-Olona-Lambro river basin and the Milan metropolitan area (northern Italy). A set of rainfall events recorded in 2023 is examined, including both stratiform and convective events. Z-R coefficients are determined using a regression-based approach following a leave-one-out methodology across events and multiple instrument pairings, to account for differences in sampling volumes and measurement characteristics.

The resulting relationships are evaluated by comparing radar-based rainfall estimates against rain gauge observations and estimates obtained using standard Z-R formulations. The analysis focuses on the performance of rainfall estimates for different methodological choices in the regression process and for stratiform and convective events, and includes an assessment of mean areal accumulated rainfall to emphasize the hydrological relevance of properly defining Z-R relationships. The study highlights the sensitivity of rainfall estimation to methodological choices in Z-R coefficient determination and underscores the importance of clearly documenting regression setups.

How to cite: Chaves González, N. A., Ceppi, A., De Michele, C., Ravazzani, G., and Cazzuli, O.: Determination of Z-R Relationships for Rainfall Estimation from Weather Radar, Rain Gauges, and Disdrometers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12024, https://doi.org/10.5194/egusphere-egu26-12024, 2026.

EGU26-12669 | ECS | PICO | HS7.1

Numerical evaluation of the wind-induced bias for the 2D Video Disdrometer 

Enrico Chinchella, Arianna Cauteruccio, Pak-Wai Chan, and Luca G. Lanza

Reconciling rainfall records from different sources, even from co-located instruments, is often difficult unless proper adjustment for instrumental and environmental sources of bias is applied. Comparisons between disdrometer and rain gauge measurements may show deviations that are usually attributed to their very different measurement principles. In this work, we show that rainfall intensity measurements from the 2D Video Disdrometer (2DVD) and a co-located tipping-bucket rain gauge can be largely reconciled once the relevant sources of bias are quantified and raw measurements are consequently adjusted.

The instrumental bias of the co-located tipping-bucket rain gauge is obtained from laboratory calibration performed at the Hong Kong Observatory (HKO). Meanwhile we rely on factory calibration for the instrumental bias of the 2DVD. Wind is assumed as the primary source of environmental bias for both instruments. Adjustment curves for the wind-induced bias of cylindrical rain gauges are here derived from existing literature (see Cauteruccio et al. 2024).

For the 2DVD, the wind-induced bias is obtained by means of numerical simulation. Using the OpenFOAM software, Computational Fluid Dynamics (CFD) and Lagrangian particle tracking simulations have been performed. CFD simulations provide the wind velocity field around the instrument body for different combinations of wind speed and direction. A k-ω SST turbulence model and a local time-stepping approach are used. Hydrometeor trajectories are modelled by numerically releasing drops ranging from 0.25 mm to 8 mm in diameter into the computational domain. The wind-induced bias is then expressed in terms of the Catch Ratio (CR), representing the ratio between the number of drops crossing both the 2DVD’s light beams in the presence of wind and their number considering undisturbed conditions.

The simulations shows that wind direction is a relevant factor since the instrument is not radially symmetric. A significant geometric shielding effect is also present and CRs may reach zero for medium to high wind speeds and small raindrop size, meaning that no drops are sensed by the 2DVD in certain conditions.

After adjustment, measurements from the 2DVD installed at the HKO’s field test site at the Hong Kong International Airport are compared against co-located rain gauge measurements. Results show an average reduction of the deviation between measurements to less than about 1 mm/h. Adjusted measurements from both instruments also report about 10% higher RI values, indicating that the raw data significantly underestimate precipitation. The adjustment procedure presented in this work is quite general and can be applied to raw measurements obtained from any 2DVD sensor if measurements from a co-located anemometer are available at the site.

Measurements obtained from the 2DVD in windy conditions should be therefore treated with caution, especially when the measured DSD is used to inform research studies on the microphysical properties of the rain process or for any comparison with other disdrometers or precipitation gauges.

References:

Cauteruccio, A., Chinchella, E., & Lanza, L. G. (2024). The overall collection efficiency of catching‐type precipitation gauges in windy conditions. Water Resources Research, 60(1), e2023WR035098. https://doi.org/10.1029/2023WR035098

How to cite: Chinchella, E., Cauteruccio, A., Chan, P.-W., and Lanza, L. G.: Numerical evaluation of the wind-induced bias for the 2D Video Disdrometer, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12669, https://doi.org/10.5194/egusphere-egu26-12669, 2026.

EGU26-13237 | PICO | HS7.1

Enhancing Rainfall Spatial Representation through Quality-Controlled Personal Weather Stations 

Jochen Seidel, Damaris Zulkarnaen, Benedetta Moccia, Elena Ridolfi, Francesco Napolitano, Fabio Russo, and András Bárdossy

The high spatial and temporal variability of precipitation, especially during short, high-intensity events, is typically not captured by rain gauge networks. Furthermore, the actual precipitation maxima do not necessarily occur at the locations of the rain gauges. This consequently leads to a systematic underestimation of interpolated precipitation amounts (Bárdossy and Anwar, 2023). Since this phenomenon depends on the sample size, i.e., the number of rain gauges, a way to increase the sample size is to use additional data of so-called opportunistic precipitation sensors. A suitable data source is provided by personal weather stations (PWS) equipped with rain gauges, which have exceeded the number of stations operated by national weather services and other authorities. They therefore offer the potential to improve quantitative precipitation estimates (Bárdossy et al. 2021, Graf et al. 2021). 

In this study, we investigate the behaviour of precipitation extremes from interpolations  in the Lazio region in Italy using different rainfall data sets. The Lazio region is characterized by a dense network of approximately 230 professionally maintained rain gauges and more than 300 Netatmo Personal Weather Stations, both providing data in  high temporal resolution Although these stations offer a valuable opportunity to enhance the spatial coverage of rainfall observations, they do not generally comply with professional standards in terms of installation, maintenance, and data reliability, and therefore require a rigorous quality control (QC) procedure. In this study, the most recent QC filters and bias correction methodologies are applied to the PWS dataset. Following the QC process, the performance of the corrected PWS observations is assessed through comparison with co-located professional rain gauges. Furthermore, the potential added value of incorporating PWS data is investigated by analyzing their contribution to the representation of rainfall spatial variability, with particular emphasis on extreme precipitation events, as well as their impact on precipitation interpolation results. The outcomes of this study aim to provide insights into the effective integration of crowdsourced weather observations into operational and research-oriented hydrometeorological applications.

References:

Bárdossy, A., Seidel, J., El Hachem, A.: The use of personal weather station observations to improve precipitation estimation and interpolation, Hydrology and Earth System Sciences, 25, 583-601, 2021. https://doi.org/10.5194/hess-25-583-2021

Bárdossy, A., Anwar, F.: Why do our rainfall–runoff models keep underestimating the peak flows? Hydrology and Earth System Sciences, 27, 1987–2000, 2023. https://doi.org/10.5194/hess-27-1987-2023

Graf, M.,  El Hachem, A., Eisele, M., Seidel, J., Chwala, C., Kunstmann, H., Bárdossy, A.: Rainfall estimates from opportunistic sensors in Germany across spatio-temporal scales. Journal of Hydrology: Regional Studies, 37. https://doi.org/10.1016/j.ejrh.2021.100883

How to cite: Seidel, J., Zulkarnaen, D., Moccia, B., Ridolfi, E., Napolitano, F., Russo, F., and Bárdossy, A.: Enhancing Rainfall Spatial Representation through Quality-Controlled Personal Weather Stations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13237, https://doi.org/10.5194/egusphere-egu26-13237, 2026.

EGU26-15175 | ECS | PICO | HS7.1

Developing a Gauge–Radar Merged Precipitation Dataset (1 hour and 1 km) for Great Britain: GRaD-GB (1H1K) 

Xiaobin Qiu, Amy C. Green, Stephen Blenkinsop, and Hayley J. Fowler

High-quality gridded precipitation datasets are essential for climate analysis and flood-risk assessment in Great Britain (GB); however, such datasets remain limited, and existing products suffer from important limitations. Rain gauge measurements provide highly accurate point-scale observations, but sparse gauge networks limit their applicability. Radar quantitative precipitation estimates (QPEs) offer useful spatial information on rainfall fields at national scale, but suffer from multiple artefacts and errors. Blended rainfall datasets therefore represent a promising approach, as they capitalise on the complementary strengths of radar and gauge observations. Accordingly, this study aims to develop a high-resolution blended precipitation dataset for GB, focusing on two key components: quality control (QC) of radar QPEs and the merging of radar and gauge rainfall.

First, radar QPEs are shown to contain substantial and spatially variable errors even after standard reflectivity-based QC. We assess the Met Office composite radar QPE for GB (hourly, 1 km resolution; 2006–2018) against approximately 1300 hourly rain gauges, demonstrating that errors increase with elevation, distance from radar, and rainfall intensity. Radar QPEs frequently underestimate high-intensity hourly rainfall and fail to detect many extreme events (≥40 mm h⁻¹), with underestimation occurring approximately 1.7 times more often than overestimation (for rainfall ≥0.2 mm h⁻¹). To address these issues, we develop a holistic, rule-based QC framework that exploits spatial–temporal continuity and rainfall-field uniqueness to further quality-control radar QPEs already processed by the Met Office. The framework (i) detects and recovers beam-blocked regions, (ii) classifies normal versus suspect rainfall fields, and (iii) identifies and replaces bad rainfall pixels associated with radar malfunction, ground clutter, and electronic noise. Application of this framework reduces the Root Mean Squared Error (RMSE) relative to gauges from 0.546 to 0.386 (−29%) and increases the correlation coefficient from 0.552 to 0.725 (+31%), while preserving genuine extreme rainfall.

Second, building on the quality-controlled radar product, we introduce a Gauss Blending Method (GBM), adapting the Gauss–Seidel method to merge radar rainfall with gauge constraints (970 gauges) and generate a spatially complete, structure-preserving hourly precipitation field at 1-km resolution. Independent evaluation using 194 gauges (2006–2018) shows that the blended product improves RMSE and mean absolute error by ~14.5% and reduces mean relative error by ~22% compared with radar-only data. The GBM also enhances rainfall detectability and outperforms commonly used adjustment approaches, including the Additive Adjustment, Multiplicative Adjustment, Mixed Adjustment, and Mean Field Bias Adjustment methods. Its overall performance is comparable to Kriging with External Drift; however, GBM shows superior performance for higher rainfall intensities (≥10 mm h⁻¹), provides substantially greater spatial data coverage, better preserves local rainfall variability, and is easier to implement in practice.

Together, the proposed QC framework and GBM enable the production of GRaD-GB (1H1K), an hourly 1-km gauge–radar merged precipitation dataset for Great Britain covering the period 2006–2023. The dataset combines hourly quality-controlled radar QPEs with hourly rainfall observations from approximately 1500 quality-controlled rain gauges. GRaD-GB (1H1K) is well suited for analysing precipitation variability, storm life cycles, and extreme rainfall, thereby providing a robust basis for hydrological applications, flood risk estimation, and extreme rainfall analysis.

How to cite: Qiu, X., C. Green, A., Blenkinsop, S., and J. Fowler, H.: Developing a Gauge–Radar Merged Precipitation Dataset (1 hour and 1 km) for Great Britain: GRaD-GB (1H1K), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15175, https://doi.org/10.5194/egusphere-egu26-15175, 2026.

EGU26-18043 | PICO | HS7.1

Urbanization and Air Pollution Effects on Precipitation Microphysics: Evidence from Disdrometer Observations in Belgium 

Armani Passtoors, Kwinten Van Weverberg, Ricardo Reinoso-Rondinel, Maarten Reyniers, Dieter Poelman, and Nicolas Ghilain

Urbanization and air pollution are increasingly recognized as important modifiers of precipitation microphysics, yet their combined influence on raindrop size distributions (DSDs) remains uncertain. This study investigates how urban land cover and particulate air pollution affect rainfall microphysical properties using multi-year disdrometer observations at three urban-edge sites near Brussels, Liège, and Ghent. Measurements from two optical laser disdrometers and one forward-scattering disdrometer are combined with ERA5 reanalysis data, Local Climate Zone (LCZ) classifications, and gridded air-quality datasets. Disdrometer data are subjected to quality control, including filtering for liquid precipitation, internal consistency checks based on rainfall rate, and comparison with nearby rain-gauge measurements. Raindrop size distributions are characterised using integral microphysical parameters, including volume mean diameter (VMD), area mean diameter (AMD), rainfall rate, reflectivity, and kinetic energy. Convective and stratiform precipitation are distinguished using reflectivity-based thresholds and variability in rainfall rate. Urban effects are quantified by relating wind-direction-dependent urban fraction to disdrometer-derived DSD parameters. Preliminary results indicate a site-dependent response of raindrop diameter to upwind urban fraction, with statistically significant positive relationships at two locations and a negative relationship at one location, highlighting the complexity and heterogeneity of urban–precipitation interactions. Seasonal stratification and wind-speed filtering do not reveal a consistent pattern across all instruments. The influence of air pollution is assessed using daily mean PM2.5 and PM10 concentrations, with initial analyses suggesting that elevated pollution levels are associated with more extreme DSD behaviour, characterised by an increased occurrence of significantly smaller and larger drop sizes compared to more narrowly distributed DSDs under cleaner conditions. Ongoing analyses further examine how these effects depend on precipitation type and how they translate into changes in rainfall kinetic energy. This work provides new observational insight into the nonlinear interactions between urban environments, aerosols, and precipitation microphysics with implications for urban hydrology, radar-based rainfall estimation, and the representation of aerosol-cloud-interactions in climate models.

How to cite: Passtoors, A., Van Weverberg, K., Reinoso-Rondinel, R., Reyniers, M., Poelman, D., and Ghilain, N.: Urbanization and Air Pollution Effects on Precipitation Microphysics: Evidence from Disdrometer Observations in Belgium, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18043, https://doi.org/10.5194/egusphere-egu26-18043, 2026.

EGU26-18161 | PICO | HS7.1

Flood forecasting based on personal weather station rainfall data 

Claudia Brauer, Jisca Schoonhoven, and Linda Bogerd

An increasing number of personal weather stations (PWSs) is installed by citizens, resulting in a large amount of real-time available precipitation data. This study assesses the applicability of these data for flood forecasting. We focussed on 30 catchments (total area 2474 km2) located in the management area of Water Board Rijn and IJssel, a water authority in the Netherlands which uses PWS data as input for their operational flood forecasting system. We compared rainfall from a network of 869 Netatmo PWSs (after applying a quality filter) and the real-time radar product from the KNMI (Royal Netherlands Meteorological Institute). Next, we used both products as input for the rainfall-runoff model WALRUS and compared the simulated discharges. These two datasets with almost no latency were validated with the final reanalysis KNMI radar product and discharge observations, for a full year (2023).

For precipitation, the real-time radar was closer to the final reanalysis radar than the PWSs in terms of Kling-Gupta Efficiency, Pearson correlation coefficient and coefficient of variation, but had a stronger negative bias. However, discharge simulations based on PWSs were closer to observations and simulations with the final reanalysis radar than simulations based on the real-time radar. This contrasting result can be explained by the bias, which was stronger for the real-time radar than for the PWSs, and is amplified in the discharge simulations due to the memory in the hydrological system. We found no clear relation between catchment size, PWS density and PWS distribution and the performance of PWS rainfall product. Reducing the density of the PWS network only led to a small deterioration in performance. The results indicate the potential of these devices to be used in hydrological applications, especially when initial hydrological model conditions are improved with data assimilation in operational flood forecasting systems.

 

 

How to cite: Brauer, C., Schoonhoven, J., and Bogerd, L.: Flood forecasting based on personal weather station rainfall data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18161, https://doi.org/10.5194/egusphere-egu26-18161, 2026.

EGU26-18992 | ECS | PICO | HS7.1

Wind effects on disdrometer measurements at different elevations along a meteorological mast 

Arianna Cauteruccio, Auguste Gires, Enrico Chinchella, and Luca G. Lanza

Disdrometers positioned at different elevations above the ground experience different wind conditions, with increasing wind velocity as the elevation increases and possibly changing wind direction. On the contrary, bulk properties of the rainfall process, such as the rainfall intensity, are not expected to change along the vertical within a limited elevation gain.

In this work, high resolution data collected over 2.5 years on a meteorological mast located at Pays d'Othe wind farm, 110 km South-East of Paris France is used. More precisely, data from an OTT Parsivel2 disdrometer, with 30 s observation time step, and a Thies Clima 3D sonic anemometer at 100 Hz, located at roughly 40 m, are used. The same setting is replicated at 80 m.

In previous research (Chinchella et al., 2025), the expected wind-induced bias of the OTT Parsivel2 disdrometer was numerically quantified using computational fluid dynamics simulation. Adjustments are here applied to raw disdrometer data depending on the measured wind speed and direction. Not only updated rain rate is provided but also the whole DSD enabling to study a few key features such as mean diameter or total concentration.

The disdrometer measurements (rain rate and DSD) at the two heights are compared before and after the correction. In a first step standard scores such as RMSE, normalized bias or Nash-Sutcliffe efficiency are used. In a second step, Universal Multifractal (UM) features are compared to get results valid, not only at a few selected scales, but across a wide range of scales. UM is a parsimonious mathematically robust framework, relying on the physically based notion of scale invariance inherited from the governing Navier-Stokes equations. It has been widely used to characterize and simulate geophysical fields extremely variable over wide range of scales such as rainfall, with the help of only 3 parameters.

This study enables to discuss the effect of the wind correction with increasing wind on the same location. It also enables to quantify the influence of wind on disdrometers measurements and retrieved UM features, an effect that has been neglected in previous investigations.

Authors acknowledge the ANR PRCI Ra2DW project supported by the French National Research Agency – ANR-23-CE01-0019-01 for partial financial support.

References

Chinchella, E.; Cauteruccio, A.; Lanza, L.G. Impact of Wind on Rainfall Measurements Obtained from the OTT Parsivel2 Disdrometer. Sensors 2025, 25, 6440. https://doi.org/10.3390/s25206440.

How to cite: Cauteruccio, A., Gires, A., Chinchella, E., and Lanza, L. G.: Wind effects on disdrometer measurements at different elevations along a meteorological mast, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18992, https://doi.org/10.5194/egusphere-egu26-18992, 2026.

EGU26-19729 | ECS | PICO | HS7.1

Large-scale Clustering of Natural Snowfall: Collective Precipitation Dynamics in Three Dimensions 

Koen Muller, Rafael Bölsterli, Sergi Gonzàlez-Herrero, Michael Lehning, and Filippo Coletti

The interactions between large collections of settling snowflakes and various turbulence intensity levels within the air column make snow precipitation difficult to forecast. Characterizing the multi-scale spatial distribution and transport of snowflakes is crucial for understanding the spatial modulations in the snow deposition process and for interpreting remote sensing signals. In this work, we perform large-scale three-dimensional tracking of snowflakes falling through the atmospheric surface layer in the Swiss Alps. We utilize a novel super-resolution field imaging system that combines 16 high-resolution cameras mounted on arrays and is flexibly deployed in ice-fishing tents at different instrumented field sites with collocated snow and wind characterization. Each camera array is fitted with shifted lenses to stitch an equivalent 100 Megapixel imaging over a 20x20 square Meter field of view at a 2-Millimeter diffraction-limited tracking resolution. Snowflakes are illuminated using white light of 5500 Kelvin at 250′000 Lumens from multiple powerful 1575 Watt stadium floodlight panels mounted on snowboards and retrofitted with lenticular lenses. Shooting data at a 150 Hertz, the system is capable of tracking millions of snowflakes over 10x10x10 cubic Meters simultaneously. We first present collective snow tracking data obtained in a mild wind vector of approximately 3 Kilometers per hour. Analyzing the fall velocity, our data suggests a multimodality for fast and slow falling snow particles, which we discuss in relation to recorded snow particle variability. Subsequently, analyzing the point-cloud data using a Voronoi tessellation, we find a predominance of clusters and voids compared to the clustering diagram for a random Poisson process. Secondly, we present field experiments being caught in a blizzard with windspeeds exceeding 30 Kilometers per hour. We first conduct a qualitative assessment of the observed patterning of snowfall in the atmosphere at high wind speeds, as well as the appearance of saltation and blowing snow layers during the field measurements. We then identify signatures of these field observations in the acquired tracking data and compare events of extreme clustering dynamics against those of the cluster diagram for the mild wind vector.

How to cite: Muller, K., Bölsterli, R., Gonzàlez-Herrero, S., Lehning, M., and Coletti, F.: Large-scale Clustering of Natural Snowfall: Collective Precipitation Dynamics in Three Dimensions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19729, https://doi.org/10.5194/egusphere-egu26-19729, 2026.

EGU26-246 | ECS | Posters on site | HS7.2

Rainfall Erosivity Estimation Accuracy and Its Impact on Soil Loss Assessments: A Case Study in Southern Italy  

Athanasios Serafeim, Andreas Langousis, Francesco Viola, Dario Pumo, Nunzio Romano, Paolo Nasta, and Roberto Deidda

Accurate and robust estimation of soil loss is essential in Mediterranean basins, where sediment transfer rates exhibit pronounced seasonal aspects driven by high-intensity storm events. While the Revised Universal Soil Loss Equation (RUSLE) is the most widely used tool for assessing soil loss, its accuracy is highly dependent on the rainfall erosivity (R-factor). This study evaluates the effect of different R-factor quantification approaches on soil loss estimates within the Tirso River basin, Sardinia’s largest basin (> 3000 km²), which provides water resources for agriculture, hydropower, and domestic supply.

We applied the RUSLE method within a geographic information system (GIS) framework. The key factors for soil erodibility (K), topography (LS), land cover-management (C), and conservation practices (P) were derived from established sources, including the European Soil Data Center, a high-resolution Copernicus DEM, the Copernicus Global Land Service, and local authorities. To estimate the R-factor, we used high-resolution (10-minute resolution) precipitation data from more than 40 rainfall gauges, applying two distinct storm identification approaches: Renard et al. (1997) and the recently developed Serafeim et al. (2025). The soil loss estimates obtained from these high-resolution methods were then compared against results derived from a suite of widely applied empirical erosivity models calibrated in Mediterranean regions. This comparative analysis reveals how relying on generalized erosivity equations can distort soil erosion assessments at the basin level.

Keywords
Soil erosion; RUSLE; rainfall erosivity uncertainty; high-resolution precipitation; sediment yield; watershed management

References

Renard, K.G., Foster, G.R., Weesies, G.A., McCool, D.K., Yoder, D.C., 1997. Predicting Soil Erosion by Water: A Guide to Conservation Planning With the Revised Universal Soil Loss Equation (RUSLE). USA, U.S, Department of Agriculture, Washington, DC.

Serafeim, A.V., R. Deidda, A. Langousis, et al., (2025) A Critical Review of Rainfall Erosivity Estimation Approaches: Comparative Analysis and Temporal Resolution Effects (To be submitted).

How to cite: Serafeim, A., Langousis, A., Viola, F., Pumo, D., Romano, N., Nasta, P., and Deidda, R.: Rainfall Erosivity Estimation Accuracy and Its Impact on Soil Loss Assessments: A Case Study in Southern Italy , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-246, https://doi.org/10.5194/egusphere-egu26-246, 2026.

Accurate precipitation estimates depend critically on the calibration fidelity of ground-based Doppler Weather Radar (DWR) systems. While these radars provide high-resolution observations essential for hydrological modelling and forecasting, their measurements often suffer from bias due to radar constant drift. Conventional calibration approaches, such as using metallic spheres, are operationally demanding and poorly maintained. As a result, biases in reflectivity can propagate, thereby degrading quantitative precipitation estimation (QPE) and introducing uncertainty into downstream applications.

This study develops a correction strategy that utilizes the well-calibrated reflectivity measurements from satellite radar (SR) to account for the systematic underestimation in ground radar (GR) measurements. A machine-learning approach based on the XGBoost algorithm is used to model the bias between GR and SR reflectivity along with key radar-geometric parameters, including range, elevation angle, and azimuth, to capture the spatial heterogeneity. The proposed framework is evaluated using eight years (2017-2024) of collocated observations from the C-band DWR at the Thumba Equatorial Rocket Launching Station (TERLS), Thiruvananthapuram, India. The proposed correction framework significantly enhances consistency between GR and SR observations. The correlation coefficient increases from 0.23 to 0.88 with a marked reduction in mean bias, mean absolute error and root mean squared error. The results demonstrate the potential of space-ground radar synergy to mitigate calibration-driven uncertainties and strengthen the reliability of near-real-time precipitation products. This framework offers a scalable pathway for enhancing operational QPE and for supporting climate-scale radar reflectivity reanalysis where long-term consistency is essential.

How to cite: Tyagi, V. and Das, S.: Correction of Systematic Calibration Drift in Weather Radar Observations to Improve Precipitation Uncertainty Modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-504, https://doi.org/10.5194/egusphere-egu26-504, 2026.

Increasing anthropogenic activities in the post-industrial era, coupled with variability in natural forcings (e.g., solar radiation, volcanic eruption) and changes in geomorphological characteristics make the climate highly non-stationary in nature. This hinders effective climate projections, adaptation and mitigation strategies for extreme weather events, hydraulic structure planning, and irrigation activity. Regionalization, which is the process of demarcating regions of similar hydroclimatic characteristics, is therefore essential for water resources planning and management. However, there are no existing approaches which take into account the non-stationarity inherent in the hydroclimatic variables (e.g., precipitation, temperature, humidity, water level) during the process of regionalization. The most widely used feature based clustering techniques involve identifying key static attributes of the hydroclimatic time series to identify dominant patterns. However, these methods often fail to capture the temporal dynamics and evolving non-stationary characteristics of the climate variables, which is a major concern in the era of climate change. To address this research gap, this study integrates two major objectives - (a) develop a novel model based regionalization procedure that accounts for non-stationarity in the hydroclimatic time series, and (b) evaluate the performance of the proposed methodology against the existing regionalization approaches using a real world case study for the Indian subcontinent. 

By coupling the Latent Gaussian State Space Models (LGSSM) with advanced fuzzy ensemble clustering techniques, the proposed methodology aims to capture this inherent non-stationarity of the hydroclimatic data, yielding better domain informed homogeneous regions. Largely used in the field of data science for future data predictions and grouping; the LGSSM model is a parametric model with sufficient flexibility which can effectively describe the non-stationary climate variables in the Euclidean Space. Further, fuzzy ensemble clustering techniques aggregate results from multiple clustering realizations, mitigating the biases inherent in any single clustering approach and incorporate fuzzy set theory by assigning membership degrees to each study area grid. Cluster validity indices such as the Dunn Index and Davies-Bouldin Index are used to find the optimal number of clusters based on intra cluster compactness and inter cluster separation. 

Hydroclimatic datasets (eg., IMD data, ERA5 reanalysis data) are obtained at 0.25x0.25 degrees spatial and daily temporal frequency for the Indian subcontinent. The methodology identified K=10 and K=6 optimum number of clusters for precipitation and temperature respectively. Final homogeneous regions are delineated by integrating topographical features such as distance from sea, elevation etc. The identified major climate regions are - (a) Northern Cold Himalayan Zone, (b) Thar Desert Area, (c) Indo-Gangetic Plain, (d) Southern Peninsular Region, (e) Western Ghats Area and (f) Dry Semi-Arid Zone. These regions are validated using regional homogeneity tests such as HoskinWallish Test. This study is the first to integrate the advanced state space modeling with fuzzy ensemble clustering for climatic regionalization, making a paradigm shift in hydrology research, from solely relying on basin-scale boundaries to an integrated approach that considers both atmospheric and physiographic boundaries. This proposed methodology provides a ready to use powerful tool for homogeneous regionalization and future projections of complex non-stationary hydroclimatic variables.

How to cite: Sengupta, D. and Vijay, S.: A Novel Framework for Homogeneous Climate Regionalisation using Advanced State Space Modeling and Ensemble Fuzzy Clustering  , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-561, https://doi.org/10.5194/egusphere-egu26-561, 2026.

Mountainous areas and the hill stations, which were traditionally considered cooler and with stable climatic conditions, are proving to mirror certain warming and changes in rainfall patterns. Considering the broader context of global climate change, this study investigates the presence of statistically quantifiable climatic shifts in the hill stations of South India by integrating observed IMD datasets with CMIP6 model simulations. An extensive bias-correction framework was employed to analyse and address the substantial systematic errors commonly associated with applying global climate models to complex terrain. The study combines established bias-correction techniques, including Quantile Mapping (QM) and Quantile Delta Mapping (QDM), with advanced machine learning algorithms such as CART, XGBoost, and a stacked ensemble model, enabling a more robust and comprehensive correction of model biases. XGBoost and the stacked model were the only approaches that demonstrated substantial improvements, showing reduced RMSE (0.55–0.76 for temperature and approximately 83–85 mm for precipitation), near-zero bias, and strong predictive skill (R² = 0.96 for temperature and NSE = 0.71 for precipitation). These models also achieved the lowest prediction uncertainty (RMSE) and the highest overall predictive performance (R²). The bias-corrected projections reveal pronounced warming across all the hill stations examined, aligning with recent evidence that traditionally cool regions are experiencing increased heat exposure. Rainfall forecasts indicate greater variability, suggesting a potential rise in both heavy rainfall events and prolonged dry spells. These findings strongly support the emerging understanding that the hill stations of South India are transitioning toward warmer and more climate-sensitive conditions. The study provides high-resolution, bias-adjusted datasets essential for climate impact assessments, tourism planning, ecosystem management, and the development of targeted adaptation policies to safeguard these vulnerable high-elevation environments.

How to cite: Devaraj, S. and Shanmugam, P. S.: Machine Learning–Enhanced Bias Correction of CMIP6 Data for Detecting Warming and Rainfall Shifts in Indian Hill Stations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-755, https://doi.org/10.5194/egusphere-egu26-755, 2026.

Precipitation drives the hydrologic cycle and directly impacts sectors from agriculture to electricity generation. However, modeling its statistical distribution is challenging. Precipitation data typically consists of frequent dry days with zero values mixed with rare, extreme events. Both ends of this spectrum can cause disasters, such as flash floods or severe droughts. In the Eastern Mediterranean, this challenge is complicated by complex topography and changing climate patterns. While machine learning (ML) models are widely used for classification or regression of the precipitation, they often treat large areas as uniform regions. However, this generalization misses important local features, such as orographic lifting along mountains or rain shadows in interior basins. Furthermore, most operational models focus only on minimizing error metrics through exact point predictions. Similar to the spatial generalization, this approach yields another problem by ignoring the forecast uncertainty, which is essential for risk-based decision-making.

This study addresses these issues by developing a spatially explicit deep learning framework based on the Probability Integral Transform (PIT). Training models on raw precipitation amounts often leads to underestimating extremes and assigning trace amounts to dry days because machine learning models tend to regress to the mean or the overrepresented classes. To solve this, the target variable (i.e., precipitation based on EOBS data) is transformed into a probability space. Each 0.1-degree pixel is normalized using its own cumulative distribution function (CDF) calculated from the 1985–2015 climatology. Here, instead of a fixed baseline assumption, the Pettitt test is applied to each pixel to detect structural breaks in the historical time series. Yet, this is applied with a condition that at least the last 10 years (2005–2015) are preserved for the CDF analysis, to ensure the approach has enough data. This ensures that the reference climatology reflects the current hydro-climatic conditions.

The deep learning model utilized in this study uses downscaled Global Forecasting System (GFS) forecasts with a 24-hour horizon. To capture the vertical structure of the atmosphere, inputs include wind components (u, v), geopotential height, and specific humidity at 500, 700, and 850 hPa pressure levels. This multi-level approach allows the model to learn the interactions between large-scale circulation, mid-tropospheric moisture transport, and low-level topographical effects. This offers a significant physical advantage over surface-only models. The study covers the period from 2015 to 2025, divided into training (2015–2020), hyperparameter tuning and validation (2020–2022), and testing (2022–2025) sets.

Finally, the deep learning model is extended with conformal prediction to bridge the aforementioned gap between statistical accuracy and yielding exact values. Unlike traditional approaches with a specific error distribution (e.g., Gaussian) assumption, conformal prediction yields distribution-free prediction intervals with a coverage guarantee. This results in adaptive confidence bounds, which can be interpreted with a widened confidence interval during unstable weather patterns and a narrowed one during stable atmospheric conditions. Consequently, the proposed approach ensures that the output is not just a forecast, but a reliable measure of its certainty across the diverse climates and topography of the Eastern Mediterranean.

How to cite: Senocak, A. U. G.: Probabilistic Precipitation Forecasting over the Eastern Mediterranean via PIT-Normalized Conformal Quantile-MOS, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1043, https://doi.org/10.5194/egusphere-egu26-1043, 2026.

Accurate precipitation estimation is of vital importance for hydrological simulation and water resources management. However, large uncertainties existed in  precipitation datasets in high-alpine regions due to the scare gauged observations and complex terrains. Data fusion technologies are widely applied to integrate advantages of multi-source precipitation datasets, but the spatial information of precipitation is usually negelected. To overcome this limitation, this study developed a two-step machine learning framework for merging multi-source precipitation datasets based on the 2D convolutional neural network (CNN) incorporating Neighboring spatial information, hereafter referred to as nCNN. The framework employs a hybrid classification-regression model to merge three gridded precipitation products (i.e., ERA5-Land, TPReanalysis and GPM) and gauged observations over a high alpine watershed in China during the period 2001-2019. Two merged precipitation datasets were generated by CNN and the proposed nCNN framework, respectively. The results show that the proposed framework effectively integrates the advantages of multiple datasets. The CNN and nCNN merged precipitation datasets have similar spatial distribution with the original products but differ in precipitation amounts. Precipitation amounts of merged data are much closer to gauged observations than original precipitation products. Both merged datasets outperform original products in terms of statistical and categorical indices evaluated based on 25 independently meteorological stations with complete time period (covering 2001-2019). However, the nCNN merged dataset exhibits superior performance over the CNN merged dataset in capturing precipitation amounts and detecting precipitation event, especially for moderate (5~10 mm/d) and heavy precipitation (>10 mm/d). Compared with the CNN merged result, the nCNN framework reduces the station-averaged root mean square error (RMSE) from 4.25 mm/d to 3.74 mm/d for moderate precipitation and from 9.43 mm/d to 8.57 mm/d for heavy precipitation, while increasing the station-averaged critical success index (CSI) by 0.03 and 0.04, respectively. Overall, this study highlights the importance of incorporating spatial information in precipitation merging, especially for high-alpine regions. 

How to cite: Li, H. and Chen, J.: A two-step machine learning framework for incorporating spatial information into multi-source precipitation merging over high-alpine regions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1833, https://doi.org/10.5194/egusphere-egu26-1833, 2026.

EGU26-1995 | Posters on site | HS7.2

Investigation of the Spatial and Temporal Variability of the Precipitation and Temperature Lapse Rates in Greece and its Application in Evaluation and Calibration of Metanalysis Meteorological Data 

Xenofon Soulis, Karampetsa Evaggelia, Konstantinos Soulis, Stergia Palli Gravani, Evaggelos Nikitakis, and Dionissios Kalivas

Accurate meteorological forcing is a prerequisite for reliable hydrological modelling, particularly in regions with complex topography like Greece. Global reanalysis datasets offer continuous coverage but often fail to capture local orographic effects when downscaled using standard, constant lapse rates. This study investigates the spatial and temporal variability of precipitation and temperature gradients across Greece and evaluates their application in calibrating reanalysis data.

We utilized a hybrid dataset comprising long-term records from 140 meteorological stations and a dense network of 777 stations for the year 2023. To process this data, we developed a specialized Python-based algorithm to estimate lapse rates and the Coefficient of Determination ($R^2$) dynamically across the domain. The methodology utilizes a "moving-window" approach, where the window dimensions and moving step were first optimized by maximizing the determination coefficient ($R^2$) to ensure statistical robustness. Using these optimized parameters, we estimated the lapse rate and $R^2$ at each grid point of the study area. Subsequently, spatial interpolations were generated to create continuous maps of vertical gradients and their statistical reliability.

The resulting spatial patterns were analyzed in relation to the country’s distinct geomorphology, including the complex coastline, the orientation of major mountain ranges (Pindos), and the insular environments. The analysis revealed that while temperature lapse rates exhibit high spatial coherence and predictability, precipitation gradients are highly sensitive to local topographic features and continentality.

These empirically derived, spatially explicit lapse rates were applied to downscale and bias-correct AgERA5 temperature and precipitation fields for the DT-Agro Digital Twin. The proposed methodology significantly reduced biases in mountainous and coastal zones compared to standard interpolation methods, demonstrating that geomorphologically informed, dynamic gradient estimation is critical for effective model calibration in data-scarce, complex terrains.

How to cite: Soulis, X., Evaggelia, K., Soulis, K., Palli Gravani, S., Nikitakis, E., and Kalivas, D.: Investigation of the Spatial and Temporal Variability of the Precipitation and Temperature Lapse Rates in Greece and its Application in Evaluation and Calibration of Metanalysis Meteorological Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1995, https://doi.org/10.5194/egusphere-egu26-1995, 2026.

EGU26-2553 | ECS | Orals | HS7.2

Change Factor Based Downscaling of Precipitation Through Neyman-Scott Rectangular Pulse based Rainfall Field Generators 

Mohammed Azharuddin, David Pritchard, and Hayley Fowler

We present a multi-site weather generator with a stochastic rainfall field generator (RFG) at its core. The weather generator is developed with the motive to produce downscaled projections for the future by utilizing the UKCP18 projections and a suite of climate models from the CMIP5/6 archive. The rainfall fields are sampled from the spatio-temporal Neyman-Scott Rectangular Pulse (NSRP) process. When considering a single site, the NSRP model parameterizes storm arrivals as a poisson process and storm separation time as exponential distribution. Each storm is assigned a certain number of raincells (a poisson random number) with each raincell having a duration and intensity which are exponentially distributed. For a multi-site model, additional considerations are made which include the radius of raincell parameterised by exponential distribution and the raincell density as a uniform poisson process (which is a replacement to the raincell generation process of single site model). The RFG has shown its efficacy in capturing the statistics of the observed rainfall across point and catchment scales which include mean monthly rainfall totals, daily variance, skewness, lag-1 autocorrelation, dry-day proportion and daily annual maximum in addition to capturing intergauge correlations. . Following the calibration and testing of the NSRP-based RFG, the other weather variables such as temperature and wind speed are ascertained through regression relationships by considering wet and dry transition states of rainfall. With the RFG established, climate model downscaling is performed by computing multiplicative and additive change factors for rainfall and temperature respectively. The RFG paramaters are perturbed by the computed change factor(s) to derive downscaled projections of precipitation thereby offering multiple plausible future scenarios in addition to a band of uncertainty associated with the projections. These projections can be further translated to hydrological responses by leveraging hydrological models thereby aiding in climate change impact assessment and adaptation.

How to cite: Azharuddin, M., Pritchard, D., and Fowler, H.: Change Factor Based Downscaling of Precipitation Through Neyman-Scott Rectangular Pulse based Rainfall Field Generators, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2553, https://doi.org/10.5194/egusphere-egu26-2553, 2026.

EGU26-2939 | Orals | HS7.2

Generation of high-resolution design rainfall using duration adjustment factors  

Hannes Müller-Thomy, Gioia Groth, Sinuhé Alejandro Sánchez Martínez, Maritza Liliana Arganis Juárez, and Kai Schröter

Temporal high-resolution design rainfall is frequently required for the dimensioning of critical infrastructure. While daily precipitation time series are generally of sufficient length to derive design rainfall for high return periods (e.g. T=100 years), the limited length of high-resolution time series often only allows for the reliable derivation of lower return periods.

Using the proposed duration adjustment factors (DAFs), design rainfall can be scaled from coarser duration levels to finer duration levels as D={5 min, 1 h}. The DAFs were derived and evaluated nationwide for Germany based on the national rainfall extreme value catalogue KOSTRA-DWD-2020 data for various durations D and return periods T (D={5 min, …, 24 h}, T={1 year, …, 100 years}). In addition, the influence of physiographic characteristics (climate zone, land use, elevation, slope, and distance to the sea) was investigated using Spearman’s rank correlation coefficient ρ for continuous variables and the effect size η² for categorical characteristics.

The DAFs depend strongly on the basis duration level (D=24 h or D=1 h) from which the scaling is applied, but show only a weak dependence on the considered return period. Elevation exhibits a weak to moderate influence, which is greater than the influence of slope and distance to the sea. Climate zone has a moderate effect on the DAFs, whereas land use exerts only a weak influence.

For 1,414 selected KOSTRA-DWD-2020 grid cells design rainfall values with D={5 min, 60 min} were generated from daily design rainfall values (D=1 day), and validated with the original high-resolution design rainfall values from the KOSTRA-DWD-2020. The impact of taking elevation into account when deriving the DAFs was examined as well. Three elevation clusters were defined, and the DAFs were derived (i) separately within each cluster and (ii) without considering clustering. Without clustering, the generation of design rainfall from an initial duration of D=1 day with T=100 years results in a relative RMSE (rRMSE) of 10 % for D=1 h, which is below the data-based uncertainty of 25 % reported by KOSTRA-DWD-2020. For D=5 min, a rRMSE of 15 % is obtained, which is slightly lower than the KOSTRA-DWD-2020 uncertainty of 18 %. Clustering leads to only a minor improvement in the median performance (considering all 1,414 grid cells), but results in a substantial reduction in the spread, i.e. the resulting uncertainties. Notably, the quality of the generated design rainfall does not deteriorate when DAFs for T=2 years are used instead of those for T=100 years, although the former can already be estimated on the basis of relatively short time series.

Consequently, the DAF approach provides a solution for deriving design rainfall for short durations and high return periods in regions where long observed daily precipitation time series are available, but only short high-resolution precipitation records exist, which is the case in most regions worldwide.

How to cite: Müller-Thomy, H., Groth, G., Sánchez Martínez, S. A., Arganis Juárez, M. L., and Schröter, K.: Generation of high-resolution design rainfall using duration adjustment factors , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2939, https://doi.org/10.5194/egusphere-egu26-2939, 2026.

EGU26-3612 | ECS | Posters on site | HS7.2

A stochastic approach for the continuous simulation of ordinary and extreme precipitation in Alpine environments 

Beatrice Carlini, Simon Michael Papalexiou, Gianluca Botter, and Francesco Marra

Predicting the impacts of climate change on hydroclimatic processes in small mountainous catchments requires long and realistic high-temporal-resolution simulations of key environmental variables, particularly precipitation, under future scenarios. Stochastic models provide an effective way to generate multi-decadal projections, but existing approaches struggle to reproduce the alternation of weather systems and sub-hourly extremes. We propose a stochastic framework that accurately describes both ordinary and extreme precipitation events, explicitly links intermittency with event inter-arrival characteristics, and represents different storm types (e.g., convective and stratiform). Our approach combines CoSMoS, which generates stochastic time series preserving probability distributions and correlation structures, with concepts from TENAX, which relates the occurrence frequency and the probability distribution of extreme precipitation to near-surface temperature. Climate change impacts are incorporated through projected changes in temperature distributions and large-scale weather patterns from regional climate models. The method is tested on the Rio Valfredda, a small Alpine catchment in the eastern Italian Alps. The sub-hourly resolution of the framework allows explicit representation of convective precipitation, a key driver of extreme events in Alpine environments.

How to cite: Carlini, B., Papalexiou, S. M., Botter, G., and Marra, F.: A stochastic approach for the continuous simulation of ordinary and extreme precipitation in Alpine environments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3612, https://doi.org/10.5194/egusphere-egu26-3612, 2026.

EGU26-4929 | Posters on site | HS7.2

How Reliable are Rainfall Observations? Assessing Credible Intervals with Bilinear Surface Smoothing 

Nikolaos Malamos, Theano Iliopoulou, Panagiotis D. Oikonomou, and Demetris Koutsoyiannis

Rainfall regionalization refers to a broader spatial modeling process that transforms point measurements into reliable continuous fields, incorporating additional information.  Yet the fidelity of the resulting continuous surface is strongly influenced by the quality of the underlying data, as well as by the density and spatial configuration of the observational network. This contribution addresses the question of how reliable rainfall data are when evaluated against a regionalized rainfall surface, by extending the Bilinear Surface Smoothing with Explanatory variable (BSSE) framework to explicitly incorporate Bayesian credible intervals.

The proposed formulation exploits the linear smoother representation of BSSE to derive the posterior covariance of the fitted bilinear surface as a function of residual variance and effective degrees of freedom. Credible intervals are obtained analytically, allowing uncertainty in variance estimation to be accounted for without resampling. Beyond quantifying uncertainty in the spatial estimates, the credible intervals provide a diagnostic measure of data reliability relative to the regionalized signal.

The extended framework is demonstrated through the regionalization of average and extreme rainfall characteristics across Greece, using ground-based observations together with elevation as explanatory variable. Stations falling outside the 95% credible interval are identified and examined, revealing that such cases frequently occur in areas with sparse gauge coverage or complex rainfall regimes. These locations highlight regions where the observational network provides limited support to the regionalized surface, leading to increased uncertainty and reduced confidence in the available data.

The analysis further reveals a strong dependence of uncertainty on temporal aggregation scale, with markedly wider credible intervals at sub-daily extremes, where station density is lowest. The BSSE methodology is implemented in a fully reproducible workflow, facilitating straightforward application of the proposed uncertainty-aware regionalization framework to other hydro-climatic datasets.

How to cite: Malamos, N., Iliopoulou, T., Oikonomou, P. D., and Koutsoyiannis, D.: How Reliable are Rainfall Observations? Assessing Credible Intervals with Bilinear Surface Smoothing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4929, https://doi.org/10.5194/egusphere-egu26-4929, 2026.

EGU26-5978 | ECS | Orals | HS7.2

Understanding the Role of Adversarial Learning in Precipitation Super-Resolution Through Explainable AI 

Shivam Singh, Simon M. Papalexiou, Hebatallah M. Abdelmoaty, Tom Hartvigsen, and Antonios Mamalakis

High-resolution precipitation information is essential for hydrological impact assessment, flood risk analysis, and the characterization of extreme events, yet climate and weather model outputs are typically available at spatial resolutions too coarse to resolve fine-scale variability. Deep-learning-based statistical downscaling has emerged as an effective approach for bridging this resolution gap; however, models trained with pixel-wise objectives often suppress spatial variability and underestimate extremes. Adversarial learning has been shown to improve the realism of downscaled precipitation fields, particularly for extreme events, but the mechanisms through which adversarial objectives influence model behavior remain insufficiently understood. In this study, we investigate how adversarial training modifies the internal representation of precipitation extremes within a super-resolution downscaling framework, using explainable artificial intelligence (XAI) as a diagnostic tool. We employ a unified U-Net architecture trained under two optimization strategies: (i) a deterministic formulation using a pixel-wise mean-squared-error loss, and (ii) an adversarial formulation in which the same U-Net generator is trained jointly with a critic through an adversarial loss. This controlled design isolates the effects of adversarial learning while holding architecture and input information constant. XAI techniques are applied to analyze differences in spatial sensitivity and attribution patterns between the two training regimes, with particular emphasis on extreme precipitation events. Rather than serving as a performance metric, XAI is used to interrogate how adversarial training reshapes the model’s reliance on spatial structure and localized variability. This work highlights the potential of XAI to provide mechanistic insight into generative downscaling models and to support more transparent evaluation of adversarial approaches for extreme precipitation.

How to cite: Singh, S., Papalexiou, S. M., Abdelmoaty, H. M., Hartvigsen, T., and Mamalakis, A.: Understanding the Role of Adversarial Learning in Precipitation Super-Resolution Through Explainable AI, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5978, https://doi.org/10.5194/egusphere-egu26-5978, 2026.

EGU26-6160 | Posters on site | HS7.2

Temporal Downscaling Using Deep Learning for Sub-hourly Time Series 

Soobin Cho, Sangbeom Jang, Jiyeon Park, and Ju-young Shin

Recent climate change has been linked to more frequent and more intense short-timescale rainfall extremes, increasing exposure to urban pluvial flooding. Because many urban catchments respond within minutes, rainfall information at sub-hourly resolution is often needed for hydrologic analyses. An AI-driven temporal downscaling approach is introduced here to derive 10-minute rainfall series from hourly observations using a conditional diffusion generative model. Rain-gauge observations at Seoul Gwanaksan (#1917), operated by the Korea Forest Service, were used. The record covers the years 2015 through 2024. Paired hourly totals and observed 10-minute series were prepared to examine whether sub-hourly rainfall sequences can be reconstructed from hourly totals while preserving realistic within-hour variability. The feasibility of loss function variation was investigated. The experiments indicate that incorporating distributional and temporal statistics into the objective function can enhance the realism of sub-hourly rainfall structure under hourly constraints. The proposed framework is expected to provide more reliable 10-minute rainfall inputs for urban hydrologic analyses and pluvial-flood–relevant applications in rapid-response catchments.

How to cite: Cho, S., Jang, S., Park, J., and Shin, J.: Temporal Downscaling Using Deep Learning for Sub-hourly Time Series, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6160, https://doi.org/10.5194/egusphere-egu26-6160, 2026.

EGU26-6400 | Posters on site | HS7.2

SEEPS4ALL: all you need to compute SEEPS (and more) when evaluating daily precipitation forecasts over Europe  

Zied Ben Bouallègue, Ana Prieto-Nemesio, Angela Iza Wong, Florian Pinault, Marlies van der Schee, and Umberto Modigliani

SEEPS4ALL [1] combines a precipitation dataset in a Zarr format and a set of verification Jupyter Notebooks for the evaluation of daily precipitation forecasts over Europe. The dataset is primarily based on daily in-situ observations from the European Climate Assessment & Dataset project (www.ecad.eu). Climate statistics are derived from long time series at each station location to enable the computation of meaningful verification metrics. For example, the Stable and Equitable Error in Probability Space (SEEPS [2]) is a score specifically designed to assess the performance of precipitation forecasts, and it requires climate statistics.

The verification notebooks showcase the computation not only of SEEPS but also of the diagonal score (the equivalent of SEEPS for probabilistic forecasts) and of the brier score as a function of climate percentiles. Finally, when comparing a gridded forecast and a point observation, one can account for observation representativeness uncertainty by dressing the forecast with pre-defined scale-dependent parametric distributions [3]. In a nutshell, SEEPS4ALL helps promote the benchmarking of daily precipitation forecasts against in-situ observations over Europe.

 

[1] Ben Bouallègue Z, A. Prieto-Nemesio, A.I. Wong, F. Pinault, M. van der Schee, and U. Modigliani (2025), SEEPS4ALL: an open dataset for the verification of daily precipitation forecasts using station climate statistics. Earth System Science Data, https://doi.org/10.5194/essd-2025-553

[2] Rodwell, M.J., D.S. Richardson, T.D. Hewson and T. Haiden (2010), A new equitable score suitable for verifying precipitation in numerical weather prediction. Q.J.R. Meteorol. Soc., https://doi.org/10.1002/qj.656

[3] Ben Bouallègue, Z., T. Haiden, N. J. Weber, T. M. Hamill, and D. S. Richardson (2020), Accounting for Representativeness in the Verification of Ensemble Precipitation Forecasts. Mon. Wea. Rev., https://doi.org/10.1175/MWR-D-19-0323.1

How to cite: Ben Bouallègue, Z., Prieto-Nemesio, A., Wong, A. I., Pinault, F., van der Schee, M., and Modigliani, U.: SEEPS4ALL: all you need to compute SEEPS (and more) when evaluating daily precipitation forecasts over Europe , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6400, https://doi.org/10.5194/egusphere-egu26-6400, 2026.

EGU26-7614 | ECS | Orals | HS7.2

Optical Flow with Recurrent All-Pairs Field Transform (RAFT) for weather radar nowcasting 

Janni Mosekær Nielsen, Michael Robdrup Rasmussen, Søren Thorndahl, Ida Kemppinen Vester, Malte Kristian Skovby Ahm, and Jesper Ellerbæk Nielsen

Weather radar nowcasting is a crucial technique in real-time urban hydrological applications, as weather radars provide spatially distributed rainfall measurements. Uncertainties in weather radar nowcasting stemming from errors in rainfall observations, motion field estimates, and rainfall evolution predictions are, however, inevitable. In this study, we implement a well-established deep learning model within computer science and image processing to estimate weather radar motion fields for nowcasting.

The deep learning model, Recurrent All-Pairs Field Transform (RAFT), developed by Teed and Deng (2020), is demonstrated to outperform several existing deep learning models for optical flow estimation. The RAFT model consists of a feature encoder that extracts features from consecutive images, a correlation layer that computes visual similarities, and a recurrent unit that iteratively updates the estimated flow field. The method is computationally efficient and highly accurate, making it relevant in real-time applications. Due to the similarities between image processing and weather radar rainfall nowcasting, the method has the potential to produce accurate motion fields for extrapolating weather radar rainfall.

In this study, three years of observation data from a Danish C-band weather radar are used to nowcast 51 rainfall events. The rainfall events consist of both linear and non-linear rainfall pattern motions. We systematically compare weather radar rainfall forecasted with Lagrangian persistence using six different motion field approaches: Global vector, COTREC (Li et al., 1995), VET (Variational Echo Tracking; Germann and Zawadski, 2002), Lucas-Kanade (Lucas and Kanade, 1981), DARTS (Dynamic and Adaptive Radar Tracking of Storms; Ruzanski et al., 2011), and RAFT.

The optical flow with RAFT is shown to statistically perform as well as the well-established methods VET and Lucas-Kanade and to outperform the global vector, COTREC, and DARTS. It is demonstrated that RAFT produces accurate and robust motion fields for both linear and non-linear rainfall motion. Thus, the RAFT model for optical flow estimation is shown to be highly relevant for weather radar nowcasting in urban hydrological applications.

References:

Germann, U., Zawadzki, I., 2002. Scale-Dependence of the Predictability of Precipitation from Continental Radar Images. Part I: Description of the Methodology. Mon Weather Rev 130, 2859–2873. https://doi.org/10.1175/1520-0493(2002)130<2859:SDOTPO>2.0.CO;2

Li, L., Schmid, W., Joss, J., 1995. Nowcasting of Motion and Growth of Precipitation with Radar over a Complex Orography. J Appl Meteorol Climatol 34, 1286–1300. https://doi.org/10.1175/1520-0450(1995)034<1286:NOMAGO>2.0.CO;2

Lucas, B.D., Kanade, T., 1981. An iterative image registration technique with an application to stereo vision, in: IJCAI’81: 7th International Joint Conference on Artificial Intelligence. pp. 674–679

Ruzanski, E., Chandrasekar, V., Wang, Y., 2011. The CASA nowcasting system. J Atmos Ocean Technol 28, 640–655. https://doi.org/10.1175/2011JTECHA1496.1

Teed, Z., Deng, J., 2020. Raft: Recurrent all-pairs field transforms for optical flow, in: European Conference on Computer Vision. pp. 402–419

How to cite: Nielsen, J. M., Rasmussen, M. R., Thorndahl, S., Vester, I. K., Ahm, M. K. S., and Nielsen, J. E.: Optical Flow with Recurrent All-Pairs Field Transform (RAFT) for weather radar nowcasting, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7614, https://doi.org/10.5194/egusphere-egu26-7614, 2026.

EGU26-7647 | ECS | Posters on site | HS7.2

Temporal Downscaling of ICON Precipitation from Hourly to 10‑Minute Resolution Using a Physically Constrained U-NET 

Midhuna Thayyil Mandodi, Caroline Arnold, Keil Paul, David Greenberg, Beate Geyer, and Stefan Hagemann

 The availability of high temporal resolution precipitation data is essential for understanding sub‑hourly hydrometeorological processes, extreme rainfall, and their impacts on hydrology and urban flooding. Especially with respect to climate change where precipitation extremes are expected to enlarge a profound data base is needed as an ensemble of downscaled climate scenarios. To store meteorological fields with high resolution in time and space is very resource demanding. The standard EURO-CORDEX dataset includes hourly precipitation data. For impact modellers however it is important to get data for the extreme events with higher resolution in time. In this study, we present a deep‑learning‑based framework to temporally downscale hourly ICON precipitation to 10‑minute resolution using a convolutional U‑Net architecture.

The source data consist of two input images corresponding to 1-hour accumulated precipitation fields. The target data are 10-minute precipitation fields derived from ICON simulations. The model is trained and evaluated over the following periods: 1980–1994 for training, 1995–1997 for validation, and 1998–1999 for testing. The model learns a mapping from the source data to the corresponding sequences of 10-minute precipitation. The U‑Net is trained to reconstruct the temporal distribution of rainfall within each hour while conserving the total hourly precipitation amount. We test the enforcement of conservation of total hourly precipitation with different techniques: a penalty term in the loss function, a constraint layer embedded into the architecture and conservation through a post-processing routine.

Model performance is evaluated using multiple statistical metrics to assess both the distribution and magnitude of precipitation. The histograms of predicted and target 10‑minute precipitation indicate that the model reproduces the marginal distribution well, while the scatter plot of total predicted versus total target precipitation summed over all grid cells and time steps shows that the model closely preserves the overall accumulated rainfall. Results also demonstrate that the U‑Net with the conservation enforcing constraint layer successfully reproduces sub‑hourly precipitation variability and captures the timing and intensity of short‑duration rainfall events more accurately than simple temporal disaggregation approaches.

This work highlights the potential of machine learning for efficient temporal downscaling of regional climate model outputs. The ultimate goal is to provide a tool for impact modelers to produce high-resolution precipitation data on their own demand . This framework has the potential to support applications in future warming scenarios. Since interested researchers can run the temporal downscaling model for their period of interest, there is no need for large memory resources to store precipitation datasets with a very high temporal resolution.

 

How to cite: Thayyil Mandodi, M., Arnold, C., Paul, K., Greenberg, D., Geyer, B., and Hagemann, S.: Temporal Downscaling of ICON Precipitation from Hourly to 10‑Minute Resolution Using a Physically Constrained U-NET, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7647, https://doi.org/10.5194/egusphere-egu26-7647, 2026.

EGU26-7985 | ECS | Orals | HS7.2

Sensitivity of Microphysical Parameters in the Thompson Scheme Using Idealized WRF Simulations 

Eulàlia Busquets, Stefano Serafin, Mireia Udina, and Joan Bech

In numerical weather prediction models, microphysics schemes represent water vapor, cloud, and precipitation processes. These schemes rely on fixed parameters that are inherently uncertain or known to vary in space and time, such as the densities of snow and graupel. Inaccurate specification of these parameters leads to errors in the partitioning of surface precipitation into liquid and ice phases. To assess the sensitivity of model results to these parameters, in this study the Weather Research and Forecast (WRF) model version 4.5 was used to perform a set of idealized two-dimensional simulations of wintertime stable orographic precipitation. The design of the experiment was inspired by observations made on 25 and 26 October 2024 on the southern slope of the Pyrenees. The model configuration includes a mountain centered in the domain with a height of 1500 m and a half-width of 10 km, a horizontal grid spacing of 1 km, and 200 vertical levels. Microphysical processes are parameterized with the Thompson scheme, which is characterized by a special snow treatment that includes snow-size distribution dependence on ice water content and temperature, and a nonspherical shape of snow particles.

Model sensitivity was assessed by running-ensemble simulations, which were created by varying 6 empirical parameters of the microphysical scheme: the exponent a in the snow mass–size relation (aₘₛ), graupel density (ρg), the shape parameter of the gamma particle size distribution for rain (μr), snow (μs), and graupel (μg), and the coefficient controlling the conversion of rimed snow to graupel (rsg). Two sets of experiments were conducted. First, 6 single-parameter perturbation experiments were run, each one with 64 members. Second, a multi-parameter perturbation experiment with 1024 members in which all parameters were perturbed simultaneously. Preliminary results indicate that cloud and snow species exhibit the strongest response to single-parameter perturbations, with particularly high sensitivity to aₘₛ and μs. Specifically, increasing aₘₛ leads to snow at higher altitudes (5000–6000 m), while increasing μs lowers the melting layer to approximately 3000 m.

This research has been funded by projects ARTEMIS (PID2021-124253OB-I00), LIFE22-IPC-ES-LIFE PYRENEES4CLIMA and the Institute for Water Research (IdRA) of the University of Barcelona.

How to cite: Busquets, E., Serafin, S., Udina, M., and Bech, J.: Sensitivity of Microphysical Parameters in the Thompson Scheme Using Idealized WRF Simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7985, https://doi.org/10.5194/egusphere-egu26-7985, 2026.

Sub-daily precipitation data are critical for continuous hydrological simulations in urban watersheds characterized by short concentration times. Unlike the widespread availability of daily precipitation data, sub-daily precipitation data are relatively limited due to the expensive monitoring instrumentation for long-term observation and high computational requirements for high-resolution simulations based on convection-permitting climate models. This study introduces a climate-informed hourly precipitation generator built on the method of fragments (MOF) framework, which accounts for both the thermodynamic influence of air temperature and the dynamic effects of atmospheric circulation patterns on sub-daily precipitation characteristics. The proposed hourly precipitation generator is extended to a multi-site configuration to preserve spatial dependencies in the simulated precipitation field. Application to stations across Germany demonstrates the effectiveness of the proposed hourly precipitation generator in reconstructing both the at-site statistical attributes and the inter-site spatial correlations. This approach provides an effective methodology for generating sub-daily precipitation inputs required for continuous hydrological modeling and flood risk assessments.

How to cite: Li, X.: A Climate-Informed Hourly Precipitation Generator Accounting for Thermodynamic and Dynamic Effects, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8527, https://doi.org/10.5194/egusphere-egu26-8527, 2026.

Downscaling of rainfall time series is the process of transforming rainfall data from a coarse temporal resolution (e.g., daily or hourly totals) into finer time scales (e.g., minutes) while preserving key statistical and physical characteristics of the original data. Downscaling techniques are widely used in hydrology, urban drainage design, flood modeling, and climate impact studies where fine-resolution rainfall data are essential for simulating hydrological response and studying the impact of extreme rainfall events.

Numerous stochastic downscaling approaches have been proposed in the literature, including point process models, random cascades, Markov chains, and weather generators, each designed to reproduce specific rainfall characteristics such as intermittency, intensity distributions, and temporal dependence. However, these methods are typically developed and evaluated independently, often using different datasets and climates, which makes it hard to assess their relative strengths and limitations.

This study presents the first joint and systematic comparison of two independently developed, state-of-the-art stochastic rainfall downscaling methods based on random cascades. Specifically, the Standard and Blunt extension cascades derived from the Universal Multifractal (UM) theory are compared with the Equal-Depth Area (EDA) approach. The methods are applied to 300 high-resolution (1-minute) rainfall events in the Netherlands and France, using increasingly challenging downscaling ratios of 4, 16, and 64. The raw data was collected with the help of optical disdrometers (OTT Parsivel2) located at three different sites.

We analyze (i) the estimation and selection of cascade generator models and their impact on performance going from event based to climatic average key parameters, (ii) the statistical properties of the downscaled rainfall time series across scales, events and cascade types, using both standard scores, quantile comparison and Universal Multifractal analysis and (iii) the relative strengths and limitations of each method in terms of ensemble spread, temporal dependence structure and extreme rainfall reproduction. By jointly evaluating multiple methods on identical datasets, we aim to advance the science behind stochastic rainfall disaggregation and lay the foundation for further model refinements and application-driven method selection.

How to cite: Schleiss, M. and Gires, A.: One Dataset, Multiple Cascades: Insights from a Joint Evaluation of Stochastic Rainfall Downscaling Methods in France and the Netherlands, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9128, https://doi.org/10.5194/egusphere-egu26-9128, 2026.

EGU26-9227 | ECS | Posters on site | HS7.2

Characterizing Global Flood Extremeness Through Physically Informed Neural Networks 

Hsiang Hsu and Hsing-Jui Wang

The tails of flood distributions provide key insights into the occurrence probability of extreme floods, which is commonly quantified by the shape parameter of an empirical Generalized Extreme Value (GEV) distribution fitted to annual maximum flood series. Despite the usefulness of fitting empirical GEV distributions to observations, considerable uncertainty remains in the estimated shape parameter across different parameter estimation approaches. In addition, most existing studies focus on regional scales, and a global-scale analysis is required to investigate the roles of varying climatic conditions and data quality in shaping extreme flood occurrence.

In this study, we first apply the L-moment method—an approach known for its robustness in extreme value statistics— to conduct a global analysis of extreme flood occurrence based on optimized GEV distributions. The Anderson–Darling test is used to evaluate the goodness-of-fit. We then integrate additional hydrological information, represented by up to 20 descriptors, into a supervised neural network (NN) model to construct a physically informed, data-driven framework for improving the estimation of GEV distribution parameters. A global-scale dataset comprising more than 6,600 river gauges, with record lengths ranging from 20 to 200 years, is used in this analysis.

Preliminary results indicate that the proposed framework can achieve flood distribution tail estimates comparable to those obtained from purely statistical methods (i.e., L-moment estimates), while providing additional physical insights into the estimation process. Overall, this study highlights the potential of integrating multi-dimensional common hydrological descriptors within a data-driven framework to support large-scale and consistent characterization of global flood extremeness.

How to cite: Hsu, H. and Wang, H.-J.: Characterizing Global Flood Extremeness Through Physically Informed Neural Networks, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9227, https://doi.org/10.5194/egusphere-egu26-9227, 2026.

EGU26-9981 | ECS | Posters on site | HS7.2

Mitigating Checkerboard Artifacts for Enhanced Precipitation Nowcasting: A Comparison of Upsampling Techniques 

Jiseong Lim, Yong Oh Lee, and Dongkyun Kim

In the field of precipitation nowcasting, the application and advancement of deep learning techniques have enabled resource-efficient predictions. In particular, U-Net variants and attention-based architectures achieve computational reduction by extracting features with wide receptive fields through downsampling and upsampling processes. However, upsampling methods can induce checkerboard artifacts when spatially adjacent pixels in high-resolution feature maps are computed from different low-resolution pixels, resulting in overlooked dependencies compared to those derived from identical pixels. This leads to discrepancies with the ground truth patterns, ultimately degrading the performance of prediction models. This paper introduces upsampling techniques known to prevent checkerboard artifacts in the super-resolution domain into precipitation prediction models, aiming to improve performance while minimizing increases in model complexity. At the upsampling stage, we incorporate sub-pixel convolution or decouple the upsampling and channel reduction processes, comparing performance against models using transposed convolution, the standard upsampling approach in U-Net. Additionally, the Checkerboard Artifacts Score (CAS) is proposed to quantify the degree of checkerboard artifacts in images, which is applied to each model for analysis. CAS is defined as the ratio of errors between pixels forming artifact boundaries to errors between all adjacent pixels. In experiments, sub-pixel convolution and the combination of nearest neighbor or bilinear interpolation with subsequent convolution record lower CAS values than transposed convolution, while also demonstrating improved performance across metrics including NSE, CSI, and RMSE. Notably, sub-pixel convolution exhibits pronounced performance with balanced POD and FAR, while the bilinear approach generates spatially natural patterns with competitive performance. Analysis of the experimental results suggests that the reduction of checkerboard artifacts contributes to performance improvement. Furthermore, this work highlights the importance of upsampling method selection in video prediction tasks and provides practical guidance for model design.

How to cite: Lim, J., Lee, Y. O., and Kim, D.: Mitigating Checkerboard Artifacts for Enhanced Precipitation Nowcasting: A Comparison of Upsampling Techniques, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9981, https://doi.org/10.5194/egusphere-egu26-9981, 2026.

EGU26-10004 | ECS | Posters on site | HS7.2

A Hybrid Bias-Correction Framework for Extreme Precipitation in Convection-Permitting Models 

Petr Vohnicky, Eleonora Dallan, Francesco Marra, and Marco Borga

Convection-permitting models (CPMs) better represent sub-daily precipitation than coarser models, but they still exhibit substantial biases in low probability occurrence extremes, with elevation-dependent patterns. In addition, the relatively short simulation periods, typically around 10 years, limit the robust estimation of rare events. This constrains the direct use of raw CPM output for applications that depend on extreme-value statistics. To address these limitations, this study introduces a hybrid bias-correction framework for CPM precipitation that targets hourly resolution.

The proposed method combines non-parametric and parametric components within an elevation-based pooling strategy. Stations and co-located CPM grid cells are grouped into elevation bands, and a common, monthly varying correction is estimated for each band to represent both spatial and seasonal variability. Low-to-moderate precipitation intensities are corrected using robust empirical quantile mapping. The upper tail is adjusted using an optimized Weibull tail model with left censoring, inspired by the Simplified Metastatistical Extreme Value approach. The optimal threshold is searched within the 0.8 to 0.97 quantile range using an adjusted Weibull tail test.

Model performance is evaluated using both extreme-value and distributional metrics derived from observations, raw CPM output, and bias-corrected series. Extreme behavior is assessed through 20-year return levels of 1-hour and 24-hour precipitation. Distributional performance is quantified using mean absolute bias computed over empirical quantiles, allowing improvements to be tracked across the full range of precipitation intensities.
Robustness is examined through a structured validation framework. Spatial robustness is tested by evaluating the elevation-based pooling approach using k-fold schemes in which subsets of stations are withheld from calibration. Temporal robustness is assessed through repeated cross-validation on the 10-year CPM slices, with six years randomly assigned to calibration and four years to validation.

Preliminary results show a reduction in mean absolute bias after correction, largely driven by an improved representation of the wet-hour ratio. When a minimum rainfall threshold is applied to the raw CPM data, the bias becomes comparable to that of the bias-corrected output, indicating that drizzle remains a key issue. For extremes, biases in 1-hour 20-year return levels generally decrease but are not fully eliminated, reflecting the large uncertainty in the distribution upper tail. For 24-hour 20-year return levels, results are mixed: biases are reduced for some CPMs but introduced or amplified for others, highlighting model-specific differences in the spatial characteristics of storm structure and organization. The validation indicates that the elevation-based pooling yields spatially robust corrections for sufficiently small, climatically homogeneous domains, while the assessment of temporal robustness remains inconclusive due to the limited length of the available 10-year CPM simulations.

How to cite: Vohnicky, P., Dallan, E., Marra, F., and Borga, M.: A Hybrid Bias-Correction Framework for Extreme Precipitation in Convection-Permitting Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10004, https://doi.org/10.5194/egusphere-egu26-10004, 2026.

EGU26-12352 | Posters on site | HS7.2

On the limitations of interchangeability between canonical and microcanonical multiplicative cascade models 

Alin Andrei Carsteanu, Stergios Emmanouil, Roberto Deidda, Anastasios Perdios, César Aguilar-Flores, and Andreas Langousis

Being the most widely used generators of multifractal measures, multiplicative cascade models have been extensively applied in the field of geophysics, and particularly in hydrometeorology. As in any modeling effort, solving the "inverse problem" is essential, and in this case, it can be described as finding the appropriate cascade model that generates a given multifractal measure. Direct measurement of a generated field (e.g., a rainfall field, or a time series thereof) results in an immediate decomposition into breakdown coefficients,  producing a microcanonical (strictly normalized) multiplicative cascade over a limited range of scales. Yet, the canonical (expectation-normalized) phenomenology at underlying scales may generate statistical properties that are non-trivial to reproduce. The present work analyzes such properties for the simplified case of a one-dimensional, beta-lognormal discrete multiplicative cascade.

How to cite: Carsteanu, A. A., Emmanouil, S., Deidda, R., Perdios, A., Aguilar-Flores, C., and Langousis, A.: On the limitations of interchangeability between canonical and microcanonical multiplicative cascade models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12352, https://doi.org/10.5194/egusphere-egu26-12352, 2026.

EGU26-13895 | Posters on site | HS7.2

A new daily gridded precipitation dataset for the island of Ireland 

Mojolaoluwa Daramola, Conor Murphy, and Peter Thorne

Reliable high-resolution precipitation datasets are essential for climate analysis, hydrological modelling, and the assessment of climate extremes. Many existing gridded rainfall products are limited by national boundaries, making it difficult to carry out consistent regional-scale climate and hydrological assessments across the island of Ireland. Here, we present a new daily gridded rainfall product developed using a homogenous methodology across the entire island of Ireland. The dataset covers the period 1980-2020 and is based on rain gauge observations from Met Éireann and UK Met Office. The gridded product is generated using a high-resolution climatological interpolation framework based on inverse distance weighting (IDW) regression, with elevation included as a covariate. This approach allows the dataset to capture fine-scale spatial variability associated with orography, while preserving daily variability and extreme rainfall events. The daily grids are first produced at 1km x 1km resolution and then resampled to a common 0.1deg x 0.1deg resolution for comparison with other gridded datasets. To assess the quality of the product, we first validate the gridded rainfall estimates using observations from a crowd-sourced citizens rain gauges from the weather observation website, providing independent evaluation of the dataset. We then evaluate the dataset through grid-to-grid comparisons with Met Éireann daily grids and other widely used regional products such as E-OBS and Multi-Source Weighted-Ensemble Precipitation (MSWEP), focusing on annual and seasonal rainfall patterns, spatial biases, and selected storm events. The new datasets provides a spatially consistent representation of daily rainfall across the island of Ireland and offers a valuable resource for climate variability studies, extreme event analysis, and hydrological applications.  

How to cite: Daramola, M., Murphy, C., and Thorne, P.: A new daily gridded precipitation dataset for the island of Ireland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13895, https://doi.org/10.5194/egusphere-egu26-13895, 2026.

EGU26-14665 | ECS | Posters on site | HS7.2

Can generative AI models downscale very rare precipitation events? An illustration of the 2020 south of France flash flood. 

Pierre Chapel, Kishanthan Kingston, Olivier Boucher, Freddy Bouchet, Kazem Ardaneh, and Redouane Lguensat

1 Introduction and objectives

Downscaling of climate model outputs is essential to correctly represent the distribution of precipitation, including extreme events which are often missed by coarse-resolution models. Deep learning approaches have shown some skills to downscale precipitation at a much lower cost than physically-based models. However, it is unclear how well they capture extreme events with decadal return periods, which only occur a few times in the training dataset. We propose to study how a diffusion-based model downscales a particularly intense precipitation episode which occurred in the South-East of France in October 2020, an event whose return period is estimated to be 100 years by Météo France [1].

2 Methods and data

Our diffusion model is based on the EDM framework from Karras et al [2]. It was trained on a domain of size 350 x 350 km² centered around Nice, France and uses precipitation and multiple covariates from the ERA5 dataset as predictors and precipitation from the regional CERRA reanalysis as predictand. An evaluation of the downscaling method using conventional ML metrics shows that our model is capable of capturing typical precipitation. To further evaluate the ability of the model to downscale very rare events, we downscaled the situation between October 2nd 06:00 UTC to October 3rd 00:00 UTC ten times using the generative capability of our diffusion-based model. The maximum six-hour accumulated precipitation registered in the CERRA dataset during this episode is above 120 mm, much more than the 99.99th percentile of the training period, which is 36 mm. We then evaluated the downscaled precipitation using CRPS, Fraction Skill Score, RAPSD, and PIT histograms [3,4], and checked the distribution of downscaled precipitation on a pixel basis as well as aggregated on hydrological basins. The diffusion model’s performance is compared to two deterministic baselines: a UNet model and a classical statistical downscaling method (bias correction spatial disaggregation) [5].

3 Results

The diffusion model is able to generate visually realistic samples for moderate precipitation events that better capture the spatial structure and distribution of precipitation than the considered baselines. When downscaling the considered extreme event, the diffusion model reproduces the position of intense precipitation, but underestimates or overestimates the intensity depending on samples (see figure). Because the event considered is exceptional in the studied dataset, it is difficult to know if this variability should be considered as an error of the downscaling model or if it is inherent to the distribution of fine scale precipitation conditioned on coarse-scale atmospheric covariates. Because samples are independent of their temporal predecessors, the 12 hour- and 24 hour-accumulated precipitation fields generated lack fine-scale details. We will investigate further this event and test ways to improve its simulation.

Figure 1. Example of four samples of downscaled six-hour accumulated precipitation fields (diffusion 0 to 5), compared to the corresponding ERA5 (low resolution) (top left) and CERRA (high resolution) (bottom left) precipitation for October 2nd, 12:00 to 18:00 UTC.

How to cite: Chapel, P., Kingston, K., Boucher, O., Bouchet, F., Ardaneh, K., and Lguensat, R.: Can generative AI models downscale very rare precipitation events? An illustration of the 2020 south of France flash flood., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14665, https://doi.org/10.5194/egusphere-egu26-14665, 2026.

EGU26-15328 | Orals | HS7.2

A framework for benchmarking precipitation type classifiers used in weather and climate models  

Ali Nazemi, Ramin Ahmadi, and Amin Hammad

Diagnosing precipitation type (ptype) is a major source of uncertainty in hydroclimatological applications. We propose a systematic framework for benchmarking the algorithms used for identifying ptype in numerical weather predictors and climate models. Six widely-used ptype algorithms, proposed by Derouin (1973), Cantin & Bachand (1993), Baldwin & Contorno (1993), Ramer (1993), Bourgouin (2000), and the European Centre for Medium-Range Weather Forecasts (ECMWF, 2024), are considered over a box region in north eastern North America with Montreal at its center. The benchmarking is made using hourly data collected at 25 Automated Surface Observing Systems during the period of 2007 to 2024. All ptype algorithms are fed by ERA5 single- and pressure-level climate reanalysis fields at 0.25° resolution. We consider four skills for benchmarking: (1) efficiency at the local scale, (2) temperature conditioning at the regional scale, as well as (3) spatial, and (4) spatiotemporal coherences. For assessing the efficiency at the local scale, we use three measures of precision, recall and F1-score that reveal how modeled ptypes are compared with observed ones at each station. For regional temperature conditioning, we extract probabilities of ptypes conditioned to near-surface temperature and compare the observed and modeled conditional density function using Kolmogorov–Smirnov test and the Wasserstein-1 (W1) distance. For both spatial and spatiotemporal coherences, we consider probabilities of co-occurrence and the Jaccard similarity index at the 0-hour time lag (spatial) and 1–48-hour lags (spatiotemporal) and quantify agreements between modeled and observed ptypes using F1-score. Our results show the excessive weakness of current ptypes algorithms in distinguishing rare and high impacts ptypes, such as freezing rain and ice pellets. Temperature conditioning show that rain, freezing rain, and ice pellets are frequently shifted toward colder regimes with W1 reaching up to 8.3 °C.  While rain classification shows moderate spatial realism, the skills in snow and freezing rain are substantially weaker. When temporal structure is added, the coherence is declined even further, with Bourgouin (2000) standing out among other algorithms with F1-score reaching to 0.5 for freezing rain and 0.61 for other/mixed types.  Our findings are a call for improving ptype algorithms in weather and climate models, particularly for predicting rare but high impact ptypes.

How to cite: Nazemi, A., Ahmadi, R., and Hammad, A.: A framework for benchmarking precipitation type classifiers used in weather and climate models , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15328, https://doi.org/10.5194/egusphere-egu26-15328, 2026.

Remote sensing technology is essential for real-time monitoring of spatiotemporal precipitation patterns. However, inherent limitations in indirect observation lead to significant errors in satellite-based precipitation products. Most existing correction methods depend on real-time ground observations, which limits their applicability for high-precision, operational use. To address this, we propose a two-stage synergistic correction framework specifically for the Global Satellite Mapping of Precipitation Near Real-Time product (GSMaP-NRT), with the goal of systematically enhancing the accuracy of its daily-scale estimates worldwide. Central to this framework is the Terrain-aware Two-stage Correction Framework (TTCF-NRT). In the first stage (historical modeling and real-time correction), we jointly utilize historical GSMaP-NRT and CPC merged precipitation data to train an improved Cumulative Distribution Function (CDF) matching model. Once trained, the model operates independently, requiring only real-time GSMaP-NRT data to perform rapid correction without needing concurrent CPC or ground-based inputs. In the second stage (near-real-time spatial refinement), we integrate the contemporaneous CPC product as a spatial reference into the first-stage corrected output. An improved Convolutional Neural Network (CNN) model, trained and validated through rigorous cross-validation, is then applied for spatial enhancement. This step significantly improves the characterization of precipitation spatial distribution, especially over complex terrain. Using the TTCF-NRT framework, we produced a daily corrected precipitation dataset for global land areas from 2020 to 2024 at a 0.5° spatial resolution. Comprehensive evaluation shows that: (1) globally, the TTCF-RT product significantly outperforms both the original GSMaP-NRT and its gauge-adjusted version (GSMaP-Gauge-NRT) in terms of Root Mean Square Error (RMSE) and Relative Bias (BIAS); (2) regionally, TTCF-NRT excels over the Continental United States (CONUS) and Western Europe. It also demonstrates consistent improvement at independent validation sites across China, though performance can still be enhanced, partly due to the limited spatial representativeness of the training data. In summary, the TTCF-NRT framework effectively combines historically calibrated real-time CDF correction with CNN-driven near-real-time spatial fusion. It offers an efficient, robust, and operationally viable correction solution for GSMaP-NNRT that does not rely on real-time external data. This approach substantially improves the accuracy and practical utility of satellite-derived precipitation estimates on a global scale, particularly in regions with complex topography.

How to cite: Wu, H.: A Terrain-Aware Two-Stage Correction Framework for Near-Real-Time Improvement of GSMaP-NRT Precipitation Estimates, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15630, https://doi.org/10.5194/egusphere-egu26-15630, 2026.

EGU26-15956 | Orals | HS7.2

Spatial-temporal modelling of convective storms with temperature-conditioned convective cell lifecycles 

Li-Pen Wang, Chien-Yu Tseng, and Christian Onof

Stochastic convective storm generators are widely used for hydrological and climate-impact applications; however, most existing methods suffer from two fundamental limitations. First, once a convective cell is sampled, its properties are typically assumed to remain constant throughout its lifetime, neglecting the intrinsic evolution of cell intensity, size, and structure during growth and decay. Second, storm events are commonly generated by repeatedly sampling cell properties from fixed distributions, which limits inter-event variability and prevents systematic modulation of storm characteristics by large-scale weather or climate conditions, despite growing evidence that convective cell properties depend on variables such as near-surface temperature.

To address these limitations, this study develops a spatial–temporal convective storm generator that explicitly represents the lifecycle evolution of individual convective cells and its dependence on temperature. Storm arrivals are described using a point-process formulation, while individual storms are modelled as clusters of rainfall cells whose intensity and geometric properties evolve dynamically through time. The temporal evolution of cell properties is governed by a copula-based lifecycle model, within which key statistical parameters are conditioned on near-surface temperature using a regression-based model. Although the temperature dependence is introduced at the level of individual cell evolution, it propagates through the generator to influence storm-scale structure and inter-event variability.

The model is calibrated using 167 convective storm events observed over the Birmingham region (UK) between 2005 and 2017, identified and tracked with a state-of-the-art storm-tracking algorithm that provides detailed information on cell tracks and physical properties, including rainfall intensity, spatial extent, lifetime, storm duration, and motion. Results show that the proposed generator more realistically reproduces observed intra-event evolution, storm-to-storm variability, and extreme rainfall behaviour than conventional generators based on stationary cell assumptions. The resulting temperature-dependent storm generator offers a computationally efficient and physically consistent alternative to convection-permitting models for applications requiring large ensembles of convective rainfall realisations.

How to cite: Wang, L.-P., Tseng, C.-Y., and Onof, C.: Spatial-temporal modelling of convective storms with temperature-conditioned convective cell lifecycles, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15956, https://doi.org/10.5194/egusphere-egu26-15956, 2026.

EGU26-16177 | ECS | Posters on site | HS7.2

Downscaling and bias-correcting satellite precipitation using a hybrid machine learning framework for flood modelling in ungauged basins. 

Hari Prakash, Pramod Soni, and Kamlesh Kumar Pandey

Hari Prakasha,  Pramod Soni b K .K Pandeyc

aResearch Scholar, Department of Civil Engineering IIT (BHU), Varanasi (U.P),221005,India,Email:hariprakash.rs.civ23@iitbhu.ac.in

bAssistant Professor,Department of Civil Engineering IIT (BHU), Varanasi(U.P),221005, India. Email: pramod.civ@iitbhu.ac.in

cAssociate Professor,Department of Civil Engineering,IIT(BHU),Varanasi(U.P),221005,India

Email: kkp.civ@iitbhu.ac.in

* Corresponding author: hariprakash.rs.civ23@iitbhu.ac.in

Accurate estimation of flood peaks in ungauged and data-scarce basins critically depends on the accuracy of rainfall inputs, still remains challenging due to the limited availability of ground observations and inherent uncertainties in satellite precipitation datas. Although datasets such as CHIRPS and GPM IMERG provide high-resolution rainfall information, their direct application in hydrological modelling is often constrained by regional bias, spatial scale mismatch, and temporal inconsistencies. Moreover, physically consistent representation of large-scale atmospheric variables is rarely incorporated in conventional bias-correction approaches.To address these limitations, this study proposes an integrated and scalable framework that combines satellite precipitation, ERA5 reanalysis variables, machine learning, and process-based hydrological modelling for flood peak estimation in ungauged basins. The framework is demonstrated over the Varuna River Basin (Varanasi, India). To resolve spatial scale mismatch, ERA5 atmospheric variables are spatially aggregated within an approximately 30 km buffer around each CHIRPS grid point prior to their use as predictors. A time-aware artificial neural network (ANN) is then developed to integrate multi-pixel GPM IMERG rainfall and aggregated ERA5 predictors, using CHIRPS as a reference dataset to generate physically informed, bias-corrected daily rainfall fields. Model robustness is ensured by systematically testing different network architectures with varying numbers of hidden neurons. The framework is implemented over more than one thousand grid cells, ensuring spatial consistency while maintaining computational efficiency.The corrected rainfall products are subsequently used to drive the SWAT hydrological model, and streamflow simulations are calibrated and validated using SWAT-CUP, with particular emphasis on reproducing peak discharge and high-flow extremes. At the daily scale, the proposed framework achieves coefficient of determination (R²) values of up to 0.76 for rainfall estimation, and leads to substantial improvements in streamflow simulation compared to uncorrected satellite rainfall, including reduced bias, improved temporal variability, and markedly enhanced simulation of flood peaks.

How to cite: Prakash, H., Soni, P., and Pandey, K. K.: Downscaling and bias-correcting satellite precipitation using a hybrid machine learning framework for flood modelling in ungauged basins., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16177, https://doi.org/10.5194/egusphere-egu26-16177, 2026.

EGU26-16535 | Orals | HS7.2

Estimates of Point Rainfall Extremes from Satellite Precipitation Products: Application and bias correction in Italy 

Cesar Arturo Sanchez Peña, Francesco Marra, and Marco Marani

Reliable estimates of extreme precipitation are essential for understanding, predicting, and mitigating natural disasters. However, global-scale assessments are limited by the sparse and uneven distribution of ground-based observations. Satellite-based rainfall products provide valuable support for extreme value analysis, but their applicability is constrained by high uncertainty and coarse spatial resolution. The coarse resolution of global datasets (100–600 km² grids) prevents direct comparison with point-scale extreme value estimates, as point and area-averaged statistics differ inherently.

This study addresses this limitation by applying a downscaling approach for extreme-value statistics based on random field theory and the Metastatistical Extreme Value Distribution (MEVD). The method exploits the autocorrelation structure of precipitation fields and is applied to each product at grid cells corresponding to rain gauge locations. Six remote sensing and reanalysis (RSR) products, along with their ensemble, are evaluated using a rain gauge network in Italy.

Downscaled estimates of daily 50-year return period precipitation are compared with corresponding estimates derived from rain gauge time series, considering both individual products and their ensemble median. To further improve the accuracy of satellite maps, two bias correction techniques are applied: quantile mapping and linear regression. The final results show that the ensemble obtained from the median of the RSR products provides the best overall performance.

This research was supported by the "raINfall exTremEs and their impacts: from the local to the National ScalE" (INTENSE) project, funded by the European Union - Next Generation EU in the framework of PRIN (Progetti di ricerca di Rilevante Interesse Nazionale) programme (grant 2022ZC2522). Marco Marani was also supported by 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: Sanchez Peña, C. A., Marra, F., and Marani, M.: Estimates of Point Rainfall Extremes from Satellite Precipitation Products: Application and bias correction in Italy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16535, https://doi.org/10.5194/egusphere-egu26-16535, 2026.

EGU26-16977 | ECS | Posters on site | HS7.2

Scale-Aware Machine Learning for Precipitation Downscaling: Impact on Regional Applications in Europe 

Hyeonjin Choi, Quyet The Nguyen, Oldřich Rakovec, Hyungon Ryu, and Seong Jin Noh

Accurate high-resolution precipitation is critical for hydrological modelling, climate impact assessment, and flood risk analysis, yet reanalysis products like ERA5 often lack the necessary spatial detail required at regional scales. This study investigates machine learning-based super-resolution techniques for precipitation downscaling, specifically examining scale-dependency and uncertainty.

We test several downscaling strategies, including convolutional neural networks with channel‑attention mechanisms and generative diffusion models. Precipitation fields are downscaled from coarse-resolution ERA5 inputs (0.25° resolution) to finer spatial resolutions using gridded observational datasets as reference: E‑OBS (0.125°) for pan‑European evaluation and, for selected regions, higher‑resolution products such as EMO‑1 (~1 km). By considering multiple scale factors, we adopt a scale‑aware framework that quantifies how downscaling skill and the associated uncertainty in super-resolution machine learning methods vary with spatial resolution and with the choice of reference dataset.

Model evaluation combines conventional accuracy metrics with diagnostics of field structure, focusing on spatial heterogeneity, intensity‑dependent behaviour (including extremes), and robustness across seasons and climatic regimes. We also discuss how scale‑dependent changes in precipitation variability and spatial structure can inform uncertainty characterisation for machine‑learning downscaling and guide its use in regional hydrological modelling and flood‑risk assessments across Europe.

How to cite: Choi, H., Nguyen, Q. T., Rakovec, O., Ryu, H., and Noh, S. J.: Scale-Aware Machine Learning for Precipitation Downscaling: Impact on Regional Applications in Europe, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16977, https://doi.org/10.5194/egusphere-egu26-16977, 2026.

EGU26-18143 | Orals | HS7.2

The sensitivity of convective precipitation in South Africa to horizontal turbulent exchange in the km-scale regional climate model REMO-NH 

Thomas Frisius, Torsten Weber, Sophie Biskop, Muhammad Fraz Ismail, and Francois Engelbrecht

This study addresses the challenges of simulating precipitation in South Africa using the convection-permitting climate model REMO-NH. In the WaRisCo project, which focuses on hydroclimatic extremes under a changing climate, a realistic representation of precipitation is essential for providing suitable forcing data for hydrological modelling. Traditional regional climate models (RCMs) with resolutions of about 11km have the limitation of not accurately reproducing extreme precipitation events such as thunderstorms. Convection-permitting RCMs (CP-RCMs) represent an alternative that offers a higher resolution and explicit simulation of convection.

For the study, the non-hydrostatic climate model REMO-NH is adopted with a resolution of about 3 km and driven by ERA5 using the double nesting technique. It enables explicit simulation of deep cumulus clouds with high vertical velocities. As entrainment of ambient air strongly influences precipitation, its representation depends critically on horizontal turbulent transfer in the model. In the standard model setup, second-order horizontal diffusion (DIFF2) takes care of this transfer. However, excessively high precipitation occurs in the autumn and winter seasons in comparison to the CHIRPS precipitation data.

A simulation with fourth order horizontal diffusion (DIFF4) reveals an even stronger precipitation bias. As an alternative to artificial diffusion, a 3D turbulence scheme has been implemented. A simulation with this scheme (TURB3D) removes this bias. Further evaluation of the results shows that the bias appears mainly for intermediate values in the frequency distribution and that the boundary layer moisture and, therefore, CAPE (convective available potential energy), are higher in the simulations with artificial horizontal diffusion. These results demonstrate that accurate treatment of 3D turbulent exchange is essential for improving convection-permitting simulations, and it will, therefore, be used for the km-scale climate projections within the WaRisCo project, which is part of the “Water Security in Africa – WASA” program.

How to cite: Frisius, T., Weber, T., Biskop, S., Ismail, M. F., and Engelbrecht, F.: The sensitivity of convective precipitation in South Africa to horizontal turbulent exchange in the km-scale regional climate model REMO-NH, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18143, https://doi.org/10.5194/egusphere-egu26-18143, 2026.

EGU26-18828 | Posters on site | HS7.2

A Novel Conditional Two-Phase Framework for High-Resolution Long-Term Precipitation Reconstruction: The Case of Sicily (1951–2025) 

Antonio Francipane, Niloufar Beikahmadi, Dario Treppiedi, and Leonardo Valerio Noto

Reliable, high-resolution gridded precipitation data are nowadays indispensable for modern climate science, hydrological modeling, and engineering applications, particularly in the Mediterranean region, where sharp topographic gradients and convective dynamics drive significant spatial variability. This study presents the development of a new daily gridded precipitation dataset for Sicily at a 2-km resolution, spanning the period 1951–2025. To address the challenges of reconstructing physically plausible fields from sparse historical records, we propose a "Conditional Two-Phase Reconstruction" framework that explicitly separates rainfall occurrence from conditional magnitude.

The methodology integrates heterogeneous in-situ observational sources, merging long-term historical archives with a modern, high-density automated rain gauge network. A core innovation of this work lies in the transfer of spatial model structures and precipitation regime definitions learned from the short-term dense network to the data-scarce historical period.

The framework first models spatial intermittency (Phase I) using regime-specific Indicator Kriging to distinguish between widespread precipitation and localized convective events. Subsequently, for magnitude estimation (Phase II), the study evaluates and implements three competing approaches: Geostatistical interpolation, hybrid Regression-Kriging utilizing Generalized Additive Models (GAMs), and Machine Learning via Extreme Gradient Boosting (XGBoost). To capture non-linear atmospheric interactions, the reconstruction leverages static physiographic predictors alongside dynamic atmospheric covariates derived from ERA5 reanalysis data, including Convective Available Potential Energy (CAPE) and Vertical Integrated Moisture Flux Divergence (VIMFD). By stratifying events into hydrometeorological regimes based on spatial coverage and intensity, the proposed framework provides a transferable blueprint for climate reconstruction in complex orographic domains. Models’ performance is evaluated through comprehensive Leave-One-Out cross validation using uncertainty and prediction error metrics.

How to cite: Francipane, A., Beikahmadi, N., Treppiedi, D., and Noto, L. V.: A Novel Conditional Two-Phase Framework for High-Resolution Long-Term Precipitation Reconstruction: The Case of Sicily (1951–2025), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18828, https://doi.org/10.5194/egusphere-egu26-18828, 2026.

EGU26-19062 | ECS | Posters on site | HS7.2

Diffusion model based downscaling of extreme precipitation in southern Europe 

Joshua Miller, Peter Watson, Kate Halladay, and Rachel James

Climate models produce enormous amounts of atmospheric data. However, these models often have very large spatial resolution, making hazard-scale, e.g. an individual city or catchment, forecasts based on future climate data impossible. Diffusion models (DMs) are a class of deep-learning generative models that can rapidly produce ensemble-like realisations of high-resolution weather states, allowing for uncertainty quantification. Numerous studies have demonstrated the efficacy of these models in faithfully downscaling weather variables from both observational datasets and from global climate models to regional climate models. However, little is known about how well DMs can perform when trained and evaluated on heterogeneous and multi-source datasets, and even less regarding their ability to faithfully emulate high-resolution extreme rainfall events. To evaluate this, we train a DM to emulate 0.1° by 0.1° hourly precipitation data from IMERG (satellite-based), using hourly 1° by 1° atmospheric fields from ERA5 (reanalysis) as the model’s input. We are also performing an out-of-distribution experiment in which extreme events are excluded from the DM’s training data in order to investigate to what extent it can accurately extrapolate to severe weather. Our domain is centred in southern Europe and was chosen to cover many diverse regions, including the Alps, Mediterranean Ocean, and northern Africa. According to continuous rank probability score, power spectral density, histograms and many other metrics, after training on balanced data our DM accurately downscales precipitation across all rainfall intensity levels, preserves fine-scale spatial structures, learns regional precipitation dynamics, and captures extreme events in the tails of the distribution. Our DM also outperforms a strong climatological baseline, and it is superior to other commonly used models such as a deterministic deep convolutional network, which tends to over-smooth and underestimate extreme events. Our results affirm the ability of diffusion models to generate robust, hazard-relevant rainfall realisations using coarse atmospheric data.

How to cite: Miller, J., Watson, P., Halladay, K., and James, R.: Diffusion model based downscaling of extreme precipitation in southern Europe, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19062, https://doi.org/10.5194/egusphere-egu26-19062, 2026.

EGU26-20546 | ECS | Orals | HS7.2

Downscaling Precipitation Projections using Generative AI: Benchmarking against the WRF Dynamical Climate Model  

Jorge Sebastián Moraga, Nans Addor, Natalie Lord, and Chris Lucas

High-resolution climate projections are essential for hydrological and meteorological impact assessments, yet dynamical numerical simulations remain computationally prohibitive for large ensembles and domains. Generative AI, specifically Probabilistic Diffusion Models (DMs), offer a promising, computationally efficient alternative. Recently, these models have demonstrated skill in reproducing historical data and serving as efficient emulators of dynamical models. The question is, therefore, whether models trained on historical observations can infer the non-stationary statistics of future climate projections.

In this work, we downscale CESM2-LENS simulations over large domains using a DM trained on reanalysis data. We investigate the model's capability to bridge the scale gap between GCM outputs (~100 km resolution) and data requirements for local hydrological impact modelling (~10 km resolution) under both historical and end-of-century scenarios. Furthermore, we compare the diffusion-based approach with the outputs of the state-of-the-art WRF dynamical model, with a focus on the changes to key hydrometeorological indices. By benchmarking DM-downscaled data against both dynamically-downscaled data and GCM baselines, we aim to assess the trade-offs between computational efficiency and physical consistency, offering insights into the generalization limits of generative AI for climate change impact studies.

How to cite: Moraga, J. S., Addor, N., Lord, N., and Lucas, C.: Downscaling Precipitation Projections using Generative AI: Benchmarking against the WRF Dynamical Climate Model , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20546, https://doi.org/10.5194/egusphere-egu26-20546, 2026.

EGU26-20641 | ECS | Orals | HS7.2

SLRainGrid-D05: High-Resolution Daily Precipitation Dataset for Sri Lanka Derived from Machine Learning and Satellite-Gauge Fusion 

Chamal Perera, Nadee Peiris, Lalith Rajapakse, Nimal Wijayaratna, and Ajith Wijemannage

Long-term, accurate fine-scale precipitation estimates are essential for hydrological and climate-related analyses, particularly in regions characterized by strong spatial rainfall variability. This study introduces SLRainGrid-D05, the first high-resolution gridded daily precipitation dataset for Sri Lanka, developed at a spatial resolution of 0.05°×0.05° and covering the entire country, including the wet, intermediate, and dry climatic zones. Sri Lanka’s tropical climate exhibits pronounced spatial variability in annual rainfall, ranging from approximately 900 mm to 5,500 mm, which cannot be adequately captured by the sparsely distributed rain-gauge network alone. In addition, satellite-based precipitation products (SPPs) are known to exhibit considerable biases over the region.

To address these limitations, a spatially consistent gridded precipitation dataset was developed by merging ground-based observations with SPPs. An initial evaluation of two widely used SPPs, IMERG and CHIRPS, demonstrated that IMERG performs better at the daily time scale, while CHIRPS shows superior performance at monthly scale. Based on these findings, daily IMERG precipitation was downscaled from its native 0.1°×0.1° resolution to 0.05°×0.05° using CHIRPS rainfall as spatial reference information. The downscaled IMERG product was subsequently merged with rain-gauge observations using machine-learning-based approaches.

The study introduces a novel hybrid merging framework that integrates graph neural networks (GNN) with inverse distance weighting (IDW) to explicitly account for the spatial autocorrelation of rainfall. The proposed method was benchmarked against conventional machine-learning models, including random forest, extreme gradient boosting, support vector machines, and artificial neural networks. Results indicate that the hybrid GNN-IDW framework consistently outperforms these benchmark methods in both rainfall detection and magnitude estimation. Specifically, it achieved the highest probability of detection (0.97) and reduced root mean square error (RMSE) and mean absolute error (MAE) by 13-41% and 9-36%, respectively, relative to the original SPPs. The SLRainGrid-D05 dataset offers a reliable, high-resolution precipitation product and represents a valuable resource for hydrological modeling, climate analysis, and improved preparedness for hydrological extremes, supporting water resources assessment and management across Sri Lanka, with the proposed methodology also being transferable to other tropical regions.

How to cite: Perera, C., Peiris, N., Rajapakse, L., Wijayaratna, N., and Wijemannage, A.: SLRainGrid-D05: High-Resolution Daily Precipitation Dataset for Sri Lanka Derived from Machine Learning and Satellite-Gauge Fusion, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20641, https://doi.org/10.5194/egusphere-egu26-20641, 2026.

EGU26-21546 | ECS | Orals | HS7.2

Benchmarking High-Resolution Quasi–Real-Time Satellite Precipitation Products over Northern Tunisia 

Abir Naceur, Hamouda Dakhlaoui, Giovanni Battista Chirico, and Anna Pelosi

Using a two-stage evaluation framework, this study evaluates five near-real-time (NRT) satellite precipitation products (GPM-IMERG V07, GSMAP V06, GSMAP V07, GSMAP V08, PERSSIAN PDIR NOW) over northern Tunisia. The evaluation is conducted at hourly temporal resolution using complementary point-to-pixel statistical analyses and hydrological modelling experiments.

The first stage consists of a comprehensive statistical assessment based on continuous, categorical, and event-based verification metrics. While continuous and categorical approaches have been widely used in previous studies, event-based evaluation methods have been applied far less frequently; their joint use in this study therefore provides a more comprehensive and complementary assessment of NRT precipitation products. 

The second stage involves a rainfall–runoff model to investigate how errors in satellite-derived precipitation propagate through the hydrological system and affect simulated streamflow.

Continuous metrics highlight considerable differences in performance among the five products. GSMaP-V8 and GPM-IMERG demonstrate the most consistent with gauge observations, followed by GSMaP-V6, with Pearson correlation coefficients (PCC) ranging from 0.32 to 0.35 and RMSE values below 0.20 mm. By contrast, GSMaP-V7 shows lower performance. PERSIANN-PDIR-NOW systematically exhibits the weakest accuracy, characterized by low correlation and large error magnitudes.

Categorical verification validates that GPM-IMERG presents the highest rainfall detection capability, achieving probability of detection (POD) values exceeding 0.45 and critical success index (CSI) values above 0.23 for light and moderate rainfall thresholds. Conversely, PERSIANN-PDIR-NOW suffers from frequent false alarms, contributing to decreased categorical skill.

Event-based analyses reveal a general tendency of satellite products to overestimate rainfall event frequency and peak characteristics. GSMaP-V8 exhibits the most balanced and consistent overall performance. GPM-IMERG and GSMaP-V6 better reproduce mean event intensity. GSMaP-V7, however, systematically overestimates event depth, intensity, and peak timing. Moreover, PERSIANN-PDIR-NOW underestimates the mean event precipitation rate, accompanied by a peak rainfall timing shifted earlier relative to observations.

The hydrological evaluation shows that rainfall–runoff modeling propagates precipitation uncertainties non-linearly into simulated streamflow. GPM-IMERG, GSMAP-V7 and GSMAP-V6 yield the most realistic flow simulations (KGE up to 0.68), Other products with comparable rainfall-level statistics nonetheless generate biased streamflow responses

Overall, the findings provide relevant information for improving NRT satellite precipitation algorithms and offer practical guidance for Community stakeholders and practitioners in selecting suitable alternative precipitation datasets in hydrological applications across specific basins, regions, or climatic zones.

 

Keywords: Hourly rainfall, Near-real-time satellite precipitation products, GPM-IMERG V07, GSMAP V06, GSMAP V07, GSMAP V08, PERSSIAN PDIR NOW, Northern Tunisia

How to cite: Naceur, A., Dakhlaoui, H., Chirico, G. B., and Pelosi, A.: Benchmarking High-Resolution Quasi–Real-Time Satellite Precipitation Products over Northern Tunisia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21546, https://doi.org/10.5194/egusphere-egu26-21546, 2026.

EGU26-21742 | ECS | Orals | HS7.2

Process-Informed Regional Climate Modeling for South Asia: The SARCI Framework 

Debi Prasad Bhuyan, Pankaj Upadhyaya, and Saroj Kanta Mishra

South Asia—home to more than a quarter of the global population—faces escalating climate risks that require scientifically credible and actionable climate information. Yet current global climate models exhibit persistent temperature and precipitation biases, reaching up to 25% and 100% of their mean values, respectively, which limits their utility for regional assessments and policy planning. To address these limitations, we develop the South Asia Regional Climate Information (SARCI) framework: a regionally optimized, process-informed system designed to improve simulations of the South Asian Summer Monsoon (SASM) and generate high-fidelity climate information.

SARCI features a customized atmospheric model based on NCAR CESM/CAM5, incorporating targeted enhancements to key physical parameterizations—stochastic entrainment for deep convection (STOCH), a dynamic convective adjustment timescale (DTAU), supplementary gravity-wave sources (GW), and region-specific similarity functions for land–air turbulent fluxes (LTF)—alongside structured parameter tuning and a statistical bias-correction and downscaling module. A systematic component-wise attribution quantifies the incremental influence of each enhancement. DTAU reduces precipitation biases and improves the annual cycle through better moisture convergence, cloud cover, and equatorial waves. STOCH and GW improve precipitation, circulation, and moisture distribution, with STOCH providing additional skill in equatorial waves. LTF primarily improves near-surface temperature with marginal precipitation benefits. Parameter tuning consolidates these gains and resolves residual inconsistencies, while the downscaling module corrects remaining magnitude errors and delivers quarter-degree, policy-relevant fields.

Together, these sequential improvements reduce longstanding SASM-related biases, yield more realistic regional circulation, and preserve acceptable global model performance. By clarifying the physical origins of model improvements and integrating co-production and regional optimization, the SARCI framework provides credible, actionable climate information for South Asia and offers a scalable pathway for other climate-vulnerable regions of the Global South.

How to cite: Bhuyan, D. P., Upadhyaya, P., and Mishra, S. K.: Process-Informed Regional Climate Modeling for South Asia: The SARCI Framework, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21742, https://doi.org/10.5194/egusphere-egu26-21742, 2026.

EGU26-2371 | ECS | Posters on site | ST2.2

Plasma Observatory's Multi-Point and Advanced Data Analysis Methods Working Group 

Giulia Cozzani, Alexandros Chasapis, and Julia Stawarz and the The Plasma Observatory Multi-Point Working Group Members and Contributors

Plasma Observatory (PO) is one of the three candidate ESA M7-class missions currently in Phase A. Its primary goal is to investigate the fundamental multi-scale processes that govern plasma energization and energy transport within Earth's magnetospheric system. To address these objectives, PO will deploy a constellation of seven spacecraft in a double-nested tetrahedral configuration with a common vertex, enabling simultaneous measurements at both fluid and ion scales and, crucially, their coupling.
Compared to previous multi-spacecraft missions such as Cluster and MMS, PO's expanded constellation introduces unprecedented opportunities to resolve multi-scale dynamics in space plasmas. However, these opportunities come with significant challenges. Realizing PO's full scientific potential requires the development and application of novel multi-point and advanced data analysis methodologies capable of exploiting measurements from more than four spacecraft.
The Multi-Point and Advanced Data Analysis Methods Working Group has been established to support the mission's Science Study Team (SST) in evaluating how PO's science goals can be achieved through its unique configuration. The Working Group brings together expertise in multi-spacecraft diagnostics and the analysis of in situ plasma observations. We present the composition and ongoing activities of the Working Group, highlight the represented analysis methods (both established and under active development), and outline ongoing efforts to assess and enhance the scientific capabilities of the PO mission.

How to cite: Cozzani, G., Chasapis, A., and Stawarz, J. and the The Plasma Observatory Multi-Point Working Group Members and Contributors: Plasma Observatory's Multi-Point and Advanced Data Analysis Methods Working Group, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2371, https://doi.org/10.5194/egusphere-egu26-2371, 2026.

EGU26-2467 | Posters on site | ST2.2

Loading non-Maxwellian velocity distributions in particle-in-cell (PIC) simulation 

Seiji Zenitani, Shunsuke Usami, and Shuichi Matsukiyo

Plasma velocity distribution functions (VDFs) exhibit many different profiles in the heliosphere. They are often loss-cone-shaped in the presence of a dipole field, they sometimes contain a power-law tail in the high-energy part, and they sometimes have ring- or shell-shaped pickup component. Particle-in-cell (PIC) simulations are useful for exploring kinetic processes, but it is not widely known how to generate such non-Maxwellian VDFs in these simulations.

In this contribution, we present Monte Carlo recipes for generating nine non-Maxwellian VDFs by using random variables. We first present two methods for the (r,q) flattop distribution. Next we present recipes for the regularized Kappa distribution. We then propose a simple procedure for the latest Kappa loss-cone model of the subtracted-Kappa distribution (Summers & Stone 2025 PoP). Properties and numerical recipes for the ring and shell distributions with a finite Gaussian width are discussed, followed by their new variants, the ring and shell Maxwellians. Finally, recipes for the super-Gaussian and the filled-shell distributions are presented.

See also: S. Zenitani, S. Usami, and S. Matsukiyo,  JGR Space Physics, in press, arXiv:2510.11890

How to cite: Zenitani, S., Usami, S., and Matsukiyo, S.: Loading non-Maxwellian velocity distributions in particle-in-cell (PIC) simulation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2467, https://doi.org/10.5194/egusphere-egu26-2467, 2026.

Non-equilibrium ionization (NEI) is a critical physical process in astrophysical environments where the plasma's thermodynamic timescales are shorter than the ionization or recombination timescales, such as in the solar wind and solar eruptions. In such rapidly evolving plasmas,  the charge states of ions are governed by time-dependent ionization equations. In this work, we report a package designed to perform fast NEI calculations using the eigenvalue method. A key feature of this package is that it can be applied in various plasma environments with arbitrary non-Maxwellian electron distributions. Furthermore, it supports both post-process analysis by tracking the movement of plasma deduced from MHD simulation and in-line calculation within MHD modeling. Finally, we show one application of this package in investigating solar wind evolution with various Kappa electron distributions. This code is freely available for download from the Web.

How to cite: Shen, C. and Ye, J.: A Package for Non-Equilibrium Ionization Simulations in Plasma with Arbitrary Electron Distributions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2866, https://doi.org/10.5194/egusphere-egu26-2866, 2026.

EGU26-3186 | Orals | ST2.2

Curlometer and gradient techniques: application to multiscale studies 

Malcolm Dunlop, Xiangcheng Dong, Huishan Fu, Xin Tan, Enze Zhao, Chao Shen, Philippe Escoubet, and Jinbin Cao

We revisit the use of multi-spacecraft techniques in range of applications applicable to close formation arrays of spacecraft, focusing on the curlometer, in particular, for both large and small-scale structures. The curlometer was originally applied to Cluster multi-spacecraft magnetic field data, but later was updated for different environments and measurement constraints such as the NASA MMS mission, with small-scale 4 spacecraft formations; the 3 spacecraft configurations of the NASA THEMIS magnetospheric mission, and derived 2-4-point measurements from the ESA Swarm mission. Spatial gradient-based methods are adaptable to a range of multi-point and multi-scale arrays and conjunctions of these, and other, missions can produce distributed, spatial coverage with large numbers of spacecraft. Four-point estimates of magnetic gradients are limited by uncertainties in spacecraft separations and the magnetic field, as well as the presence of non-linear gradients and temporal evolution (giving certain applicability limits which can be mitigated by supporting information on morphology. Many magnetospheric regions have been investigated directly (illustrated here by the magnetopause, ring current and field-aligned currents at high and low altitudes). In addition, the analysis can support investigations of transient and smaller-scale current structures (e.g. reconnected flux tubes, boundary layer sub-structure, or dipolarisation fronts) and energy transfer processes. We anticipate the use of complementary information from imminent missions such as SMILE and the new EISCAT-3D radar.

How to cite: Dunlop, M., Dong, X., Fu, H., Tan, X., Zhao, E., Shen, C., Escoubet, P., and Cao, J.: Curlometer and gradient techniques: application to multiscale studies, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3186, https://doi.org/10.5194/egusphere-egu26-3186, 2026.

EGU26-3438 | Posters on site | ST2.2

Fluxgate Magnetic Field Instrument for Seven Small Plasma Observatory Spacecraft 

Evgeny V. Panov, Ferdinand Plaschke, Lorenzo Matteini, David Fischer, Gerlinde Timmermann, Patrick Brown, Hans Ulrich Auster, Emanuele Cupido, Werner Magnes, Rumi Nakamura, Yasuhito Narita, Ingo Richter, Adriana Settino, Zoltan Vörös, and Owen Roberts

The fluxgate magnetic field instrument (MAG) onboard seven small Plasma Observatory (PO) spacecraft is a collaborative effort between the Space Research Institute in Graz (AT), the Technical University of Braunschweig (DE) and the Imperial College London (UK). MAG is a dual-sensor fluxgate magnetometer that measures the vector of the magnetic field in space. The science objective of MAG is to provide the magnetic field measurements that are crucial for analyzing plasma processes in six key science regions of Plasma Observatory: foreshock, bowshock, magnetosheath, magnetopause, transition region and tail current sheet. MAG measures the background magnetic field in the near-Earth space in the range ± 10,000 nT with frequencies up to 256 Hz, a noise floor of less than 10 pT/√Hz at 1Hz and an error of less than ±0.5 nT.  The targeted value range in terms of static and variational field for PMO is in the order of 100 nT. The maximum sampling frequency of 256 Hz allows for a sufficient overlap with concurrent Search Coil Magnetometer measurements. The poster gives an overview over the magnetometer design as well as its scientific goals.

How to cite: Panov, E. V., Plaschke, F., Matteini, L., Fischer, D., Timmermann, G., Brown, P., Auster, H. U., Cupido, E., Magnes, W., Nakamura, R., Narita, Y., Richter, I., Settino, A., Vörös, Z., and Roberts, O.: Fluxgate Magnetic Field Instrument for Seven Small Plasma Observatory Spacecraft, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3438, https://doi.org/10.5194/egusphere-egu26-3438, 2026.

EGU26-3463 | Posters on site | ST2.2

Science Study Team Working Groups of the ESA M7 Mission candidate Plasma Observatory  

Matthew Taylor and the Plasma Observatory Science Study Team Working Group Leads

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, with potential down selection to Phase B in Summer 2026. 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. In addition an Early Career Researcher network has been set up.

This paper provides an overview of these entites and how you can get involved in Plasma Observatory.

How to cite: Taylor, M. and the Plasma Observatory Science Study Team Working Group Leads: Science Study Team Working Groups of the ESA M7 Mission candidate Plasma Observatory , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3463, https://doi.org/10.5194/egusphere-egu26-3463, 2026.

EGU26-3730 | ECS | Posters on site | ST2.2

Simulations of Plasma Observatory's Energetic Particle Experiment 

Hannes Ebeling, Svea Jürgensen, Christopher Liu, Patrick Kühl, Lars Berger, Robert F. Wimmer-Schweingruber, Vassilis Angelopoulos, Ethan Tsai, Ryan Caron, Colin Wilkins, Malcolm W. Dunlop, Demet Ulusen Aksoy, Mark Prydderch, Alex Steven, Rami Vainio, and Jussi Lehti

Plasma Observatory is a candidate for the European Space Agency's upcoming M7 science mission. It will investigate how particles are energized in space plasmas and how energy is transported across different scales and regions of the Earth’s magnetosphere. For this, the Energetic Particle Experiment (EPE) provides electron and ion measurements in the energy range from 30 to 600 keV, with an optional extension of measurements down to around 20 keV for electrons and ions and up to 1.5 MeV for ions. Both electron and ion measurements have an energy resolution of 20 % or better. The design of the EPE is based on the well-proven magnet-foil technique and features two geometrical factors for both electrons and ions in order to increase the dynamic range of observable fluxes.

To validate and demonstrate the EPE's capabilities, GEANT4 Monte Carlo simulations of the current instrument design were performed, which allowed to derive the geometrical factors and energy-dependent responses to electrons and protons. Based on these results, the instrument’s performance in the expected particle flux environments during the Plasma Observatory mission were investigated.

How to cite: Ebeling, H., Jürgensen, S., Liu, C., Kühl, P., Berger, L., Wimmer-Schweingruber, R. F., Angelopoulos, V., Tsai, E., Caron, R., Wilkins, C., Dunlop, M. W., Ulusen Aksoy, D., Prydderch, M., Steven, A., Vainio, R., and Lehti, J.: Simulations of Plasma Observatory's Energetic Particle Experiment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3730, https://doi.org/10.5194/egusphere-egu26-3730, 2026.

EGU26-3810 | ECS | Orals | ST2.2

The Lorentz Electron and Ion Analyser (LEIA) – An Instrument Prototype for Low-Contamination Particle Measurements 

Svea Jürgensen, Hannes Ebeling, Lars Berger, Patrick Kühl, Robert F. Wimmer-Schweingruber, Lars Seimetz, Stephan Böttcher, Björn Schuster, Malcolm Wray Dunlop, Rami O Vainio, Vassilis Angelopoulos, and Ethan Tsai

Plasma Observatory is a candidate mission of the European Space Agency (ESA), with a potential launch in 2037. It aims to investigate plasma coupling across multiple scales in the Earth’s magnetosphere.

Energetic ions and electrons are sensitive tracers of plasma acceleration and transport processes. This makes high-cadence in situ measurements essential for understanding magnetospheric dynamics. On Plasma Observatory, such measurements will be provided by the Energetic Particle Experiment (EPE). The instrument utilizes the well-proven foil–magnet technique to separate electrons from ions and covers an energy range from 30 keV to 600 keV.

In this contribution, we present a novel instrument prototype, the Lorentz Electron and Ion Analyser (LEIA). The concept is based on an earlier, alternative design developed in the context of Plasma Observatory, but is independent of the currently baselined EPE instrument and not intended for flight on Plasma Observatory. It uses a single-channel approach, separating particles by means of a finely tuned magnetic field as well as a modified dE/dx-E detector stack. No foil is used.

This design aims to enable advanced particle species discrimination while significantly reducing electron–ion cross-contamination. Although LEIA is presented as a concept study rather than a mission-specific instrument, it demonstrates a promising pathway for future energetic particle measurements in magnetospheric and heliospheric science missions.

How to cite: Jürgensen, S., Ebeling, H., Berger, L., Kühl, P., Wimmer-Schweingruber, R. F., Seimetz, L., Böttcher, S., Schuster, B., Dunlop, M. W., O Vainio, R., Angelopoulos, V., and Tsai, E.: The Lorentz Electron and Ion Analyser (LEIA) – An Instrument Prototype for Low-Contamination Particle Measurements, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3810, https://doi.org/10.5194/egusphere-egu26-3810, 2026.

We propose and verify a new statistical topology framework to study the complex magnetic field evolution of Sun-like stars, and energy outbursts in power-law probability distributions. This new framework consider self-similar topological structures as a statistical ensemble, and derive new power-law scalings for fundamental quantities such as magnetic flux, helicity, and energy in outbursts. This new framework not only successfully predicts magnetic emergence on the Sun, but also shed light on the coronal heating problem by reconciling the nanoflare theory with previous challenging observations. Part of this presenatation is published as (Xiong et. al., ApJ, 2025), while part of the work is still under consideration by journal publication by the time of this abstract submission.

How to cite: Xiong, A. and Yang, S.: New Statistical Topology Theory Predicts Turbulent Magnetic Emergence and Energy Outburts, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6240, https://doi.org/10.5194/egusphere-egu26-6240, 2026.

EGU26-6528 | ECS | Posters on site | ST2.2

Machine-learning-based closures for the 10-moment fluid model 

Sophia Köhne, Simon Lautenbach, Emanuel Jeß, Rainer Grauer, and Maria Elena Innocenti

Many plasma phenomena involve physical processes spanning a wide range of spatial and temporal scales. Accurately capturing such multi-scale dynamics with fully kinetic simulations quickly becomes computationally prohibitive. Fluid models therefore remain an essential tool, but their applicability depends critically on the order at which the hierarchy of moment equations derived from the Vlasov equation is truncated and on the assumptions used to approximate neglected higher-order moments. Extended fluid models such as the 10-moment system therefore require appropriate closures to account for kinetic effects encoded in higher-order moments, such as the heat flux.

In this work, we develop data-driven closures for the 10-moment fluid model based on machine learning (ML). Using supervised learning, the ML models learn to predict the six independent components of the divergence of the heat flux tensor from lower-order moments and the electromagnetic fields. The models are trained on data obtained from two-dimensional fully kinetic Vlasov simulations of magnetic reconnection in a Harris current sheet with varying guide field strength, performed with the muphy 2 code (Allmann-Rahn et al., 2023).

We compare different machine learning architectures, including classical multilayer perceptrons (MLPs), fully convolutional networks, and Fourier Neural Operators (FNOs), assessing their ability to capture spatially structured kinetic effects across different physical regimes. The models are evaluated in terms of accuracy, generalization across guide field conditions, and their suitability for incorporation into fluid simulations. Our results highlight the potential of operator-learning approaches for constructing robust, data-driven closures and provide insight into the strengths and limitations of different ML strategies for plasma fluid modeling.

How to cite: Köhne, S., Lautenbach, S., Jeß, E., Grauer, R., and Innocenti, M. E.: Machine-learning-based closures for the 10-moment fluid model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6528, https://doi.org/10.5194/egusphere-egu26-6528, 2026.

EGU26-7134 | ECS | Posters on site | ST2.2

Improved Design of Fluxgate Magnetometer Electronics for Geospace Observation 

Gerlinde Timmermann, David Fischer, Christoph Poetzsch, Olaf Hillenmaier, Evgeny Panov, Ingo Richter, Hans-Ulrich Auster, and Ferdinand Plaschke

In the last decades, magnetometers have been an important part of scientific space explorations, giving insights in the behavior of space plasmas and how they change throughout the solar system. We plan to contribute a fluxgate magnetometer for the Plasma Observatory Mission, which is an M7 candidate of ESA for making multi-point measurements in Earth's magnetosphere. This magnetometer builds on a heritage design that was already used on missions like Rosetta, BepiColombo, and JUICE. The next design iteration of the electronics introduces improvements in the feedback loop, making feedback faster and better adjusted to the currently measured values. This poster shows how the new design works and first measurements of the new electronics.

How to cite: Timmermann, G., Fischer, D., Poetzsch, C., Hillenmaier, O., Panov, E., Richter, I., Auster, H.-U., and Plaschke, F.: Improved Design of Fluxgate Magnetometer Electronics for Geospace Observation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7134, https://doi.org/10.5194/egusphere-egu26-7134, 2026.

EGU26-7791 | ECS | Posters on site | ST2.2

Exploring the response of planetary magnetospheres to intense space weather events 

Lorenzo Biasiotti and Stravro Ivanovski
Extreme Space Weather (SWE) events have a crucial role in shaping the dynamics of Earth's magnetospheric boundary layer. Under such conditions, several plasma processes can be triggered, including the Kelvin-Helmholtz instability (KHI). This instability arises from the velocity shear at the boundary of two regions: the nearly stagnant magnetosphere (MSP) and the anti-sunward streaming magnetosheath (MSH).

KHI can grow into finite-amplitude Kelvin–Helmholtz waves (KHWs), which may subsequently roll-up into large-scale vortices (KHVs). These vortices can twist magnetic field lines and trigger vortex-induced tearing mode instability (TMI). In the context of planetary magnetospheric dynamics, such instabilities are fundamental because they (i) drive substantial mass, energy, and momentum transport from the MSH into the MSP; (ii) generate ultra-low-frequency magnetospheric waves; and (iii) drive field-aligned currents coupling to the ionosphere.

In this work, we analyze two SWE events that occurred in January and November 2025, during which the Sun produced some of the strongest flares of Solar Cycle 25, associated with Earth-directed coronal mass ejections (CMEs). Our study combines in-situ magnetospheric observations from MMS and THEMIS with ionospheric measurements from Swarm. Furthermore, we employ our two-dimensional magnetohydrodynamic (MHD) model (Ivanovski et al. 2011; Biasiotti et al. 2024) to characterize the flow dynamics within the magnetopause mixing layer in the fluid limit.

Finally, we analyze predictions of solar activity for May 2039, the expected operational window of the proposed Plasma Observatory (PO) mission, to identify analogue intervals representative of the SWE conditions likely to be encountered by PO. We also examine the orbits of THEMIS, MMS, and Cluster to search for comparable magnetopause crossings. Our results indicate that the orbital configuration of PO would enable continuous monitoring of the dawnside magnetopause for 10-12 days, allowing the full evolution of KH vortices and their interaction with TMI to be captured. This represents a unique capability compared with current missions, which observe such processes only during brief and sporadic crossings.  

This research has been carried out within the framework of the Space It Up project funded by the Italian Space Agency, ASI, and the Ministry of University and Research, MUR, under contract n. 2024-5-E.0 - CUP n. I53D24000060005.

How to cite: Biasiotti, L. and Ivanovski, S.: Exploring the response of planetary magnetospheres to intense space weather events, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7791, https://doi.org/10.5194/egusphere-egu26-7791, 2026.

Quasi-periodic pulsations (QPPs) at sub-second periods are frequently detected in the time series of X-rays and radio emissions during stellar flares, and they can be seen in solar radio emissions. However, such short-period QPPs are rarely reported in the hard X-ray (HXR) emission of solar flares. We explored the QPP patterns at short periods in HXRs, γ-ray continuum and radio emissions produced in two solar flare on 2024 October 03 (X9.0) and 2025 January 19 (C8.2). The short period at about 1 s is simultaneously observed in wavebands of HXR and γ-ray continuum during the X9.0 flare, and the restructured images show that the HXR sources move significantly during the short-period QPP, suggesting that the short-period QPP may be caused by the interaction of hot plasma loops that are rooted in double footpoints. The similar short-period QPP is also detected in wavebands of HXR and low-frequency radio emission during the impulsive phase of a C8.2 flare, which could be associated with non-thermal electrons that are periodically accelerated by the intermittent magnetic reconnection.

How to cite: Li, D.: Detection of short-period pulsations in solar hard X-ray and radio emissions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8951, https://doi.org/10.5194/egusphere-egu26-8951, 2026.

EGU26-9730 | ECS | Posters on site | ST2.2

Quantification of non-Maxwellian properties in plasma mixing during magnetopause reconnection 

Ivan Zaitsev, Konstantinos Papadakis, Markku Alho, Sanni Hoilijoki, Urs Ganse, Teemu Roos, and Minna Palmroth

We investigate ion velocity-space dynamics within the exhaust region of asymmetric magnetopause reconnection using global hybrid-Vlasov simulations. To quantify the complexity of velocity-space structures arising from the mixing of magnetospheric and magnetosheath ion populations, we employ the Hermite transform and Gaussian Mixture Model (GMM) analyses. In the Hermite representation, we use a fixed number of 22 harmonics to ensure computational feasibility. From this expansion, we compute a scalar measure of enstrophy—the total power contained in the non-zero Hermite modes—which characterizes the available free energy in the system. For the GMM approach, we test different numbers of ion populations and evaluate the corresponding multi-beam thermal energy for each decomposition. We further define the thermal energy drop as the relative difference between the thermal energy of an equivalent single-Maxwellian distribution and the total multi-beam thermal energy. Both enstrophy and thermal energy drop diagnostics (for any number of beams considered) exhibit consistent trends during the phase of plasma thermalization and anisotropic acceleration, demonstrating that the redistribution of thermal energy can be effectively captured even with a limited number of Hermite modes.

How to cite: Zaitsev, I., Papadakis, K., Alho, M., Hoilijoki, S., Ganse, U., Roos, T., and Palmroth, M.: Quantification of non-Maxwellian properties in plasma mixing during magnetopause reconnection, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9730, https://doi.org/10.5194/egusphere-egu26-9730, 2026.

EGU26-10219 | ECS | Posters on site | ST2.2

Statistical Maps of Foreshock Waves Utilising 23 Years of Cluster Data 

Rose Atkinson, Heli Hietala, Davide Manzini, David Burgess, and Tomas Karlsson

Ultra-low frequency (ULF) magnetosonic waves arise from the backstreaming ion population in the quasi-parallel foreshock region, participating in several key foreshock processes such as particle acceleration and shock reformation both directly and by steepening into transient structures such as SLAMS (short, large-amplitude magnetic structures). To better understand the effects of upstream solar wind conditions on these multi-scale processes, we use the 23-year Cluster dataset to study ULF waves under a range of solar wind conditions, combining Cluster data with the upstream OMNI product to produce Geocentric Interplanetary Medium (GIPM) coordinate mappings of foreshock wave properties. This method enables us to compare foreshock observations across changing solar wind conditions, by accounting for the changes in foreshock location and scale with varying IMF direction and dynamic pressure. We present the first quantitative maps of compressive and transverse foreshock wave power as a function of cone angle and Mach number, and study the ULF wave power dependence on Mach number, solar wind speed, density and background magnetic field strength, finding a slight increase in normalised foreshock wave power with increasing Mach number. We find the magnetic field strength to be the strongest determinant of foreshock wave power: wave power increases with decreasing field strength. The solar wind speed and density play more minor roles. We find that the relative changes in ULF-band power in the pristine solar wind are larger than in the foreshock under changing solar wind conditions. In the magnetosheath, we find higher ULF-band wave power on the quasi-parallel side, compared to quasi-perpendicular. These results set the context for future missions investigating waves in the solar wind, foreshock, and the magnetosheath, such as HelioSWARM and Plasma Observatory.

How to cite: Atkinson, R., Hietala, H., Manzini, D., Burgess, D., and Karlsson, T.: Statistical Maps of Foreshock Waves Utilising 23 Years of Cluster Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10219, https://doi.org/10.5194/egusphere-egu26-10219, 2026.

EGU26-10302 | Orals | ST2.2

Interlinked Spatiotemporal Patterns of Magnetospheric Lower-Band Whistler Mode Waves  

Ondrej Santolik, Ivana Kolmašová, Ulrich Taubenschuss, and Miroslav Hanzelka

Natural electromagnetic wave emissions of lower-band chorus and exohiss affect energetic electron populations in the Earth's outer radiation belt. Despite extensive studies, the spatiotemporal  characteristics of amplitude distributions of these whistler-mode waves remain incompletely characterized. We analyze nearly seven years of Van Allen Probes data combined with over nineteen years of Cluster spacecraft measurements to quantify these distributions. We find that distributions of wave amplitudes exhibit a wide and approximately log-normal core with a variable heavy tail, both dependent on geomagnetic activity and position, while time intervals between detections follow a power-law distribution indicative of temporal clustering. Intense waves occurring predominantly near the postmidnight equatorial region have average intervals of tens of minutes to hours between their detections. These findings suggest that the bursty nature of whistler-mode waves may not be fully captured by long-term averages, which are commonly used in models of radiation belt electron dynamics.

How to cite: Santolik, O., Kolmašová, I., Taubenschuss, U., and Hanzelka, M.: Interlinked Spatiotemporal Patterns of Magnetospheric Lower-Band Whistler Mode Waves , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10302, https://doi.org/10.5194/egusphere-egu26-10302, 2026.

EGU26-10374 | Orals | ST2.2

Cluster mission: why do we still need to calibrate instruments after 25 years? 

Arnaud Masson and Philippe Escoubet

The Cluster mission holds a unique place in space science history: it was the first-ever fleet of four spacecraft flying together in the Earth’s magnetosphere. But its legacy goes far beyond that, it set a new benchmark for data calibration, a cornerstone of its scientific success.

Launched in 2000, each spacecraft carried 11 identical instruments. Remarkably, most of these instruments were still operating until the end of operations, late September 2024. Some showed almost no degradation after nearly 25 years in space, while others naturally experienced reduced sensitivity over time.

To achieve the highest possible data quality, Cluster PI teams employed advanced calibration methods, intertwined instrument calibration procedures, and even machine learning techniques. In this presentation, we will showcase a selection of examples drawn from the latest technical reports on these calibration efforts, gathered in a special issue of JGR Space Physics, to be published in 2026.

How to cite: Masson, A. and Escoubet, P.: Cluster mission: why do we still need to calibrate instruments after 25 years?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10374, https://doi.org/10.5194/egusphere-egu26-10374, 2026.

EGU26-10382 | ECS | Orals | ST2.2

Ion Energization and Acceleration Associated with Foreshock Bubbles: Results from a Hybrid-Vlasov Simulation and MMS Observations 

Souhail Dahani, Lucile Turc, Veera Lipsanen, Shi Tao, Jonas Suni, Yann Pfau-Kempf, Milla Kalliokoski, Minna Palmroth, Daniel Gershman, Roy Torbert, and James Burch

Foreshock Bubbles (FBs) are large-scale transient structures found in Earth's foreshock region and are associated with foreshock-discontinuity interaction. FBs play a significant role in accelerating and energizing plasma through various mechanisms. In this study, we investigate the contribution of FBs to ion acceleration and energization by analyzing the key energy terms found in the equations that describe the temporal evolution of the kinetic and internal energy densities, namely, the pressure gradient term, the electromagnetic term and the pressure-strain term. To carry out this study, we employ the global hybrid-Vlasov simulation Vlasiator and compare our results with in-situ observations from the Magnetospheric MultiScale (MMS) mission. We find that FBs exhibit distinct signatures in the energy terms throughout their life cycles, from formation to decay as they interact with the bow shock. We show that the evolution of FBs involves complex energy conversions between electromagnetic, kinetic, and thermal energies. Notably, the energy term magnitudes increase during the initial phase of the FB, reach a peak, and subsequently decline as the FB dissipates, in agreement with previous studies. We find also strong energy conversion at the interface between the FB core and compressed edge due to the presence of a current sheet highlighting the complex contributions of the FB in accelerating and energizing ions.

How to cite: Dahani, S., Turc, L., Lipsanen, V., Tao, S., Suni, J., Pfau-Kempf, Y., Kalliokoski, M., Palmroth, M., Gershman, D., Torbert, R., and Burch, J.: Ion Energization and Acceleration Associated with Foreshock Bubbles: Results from a Hybrid-Vlasov Simulation and MMS Observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10382, https://doi.org/10.5194/egusphere-egu26-10382, 2026.

EGU26-10626 | Posters on site | ST2.2

The Plasma Observatory Ion and Mass Composition Analyzer [IMCA] 

Maria Federica Marcucci and the The Plasma Observatory IMCA Team

Plasma Observatory (PO) is the first multiscale mission tailored to study plasma energization and energy transport in the Earth's Magnetospheric System through simultaneous measurements at both ion and fluid scales. PO consists of seven identical small satellites (Sister SpaceCraft, SSC) that move on an equatorial elliptical orbit with an apogee of ~17 and a perigee of ~7 Earth radii in a two tetrahedra with a common vertex formation. The payload on board the SSCs give a full characterization of the plasma at the ion and fluid scales in the key science regions:  bow shock, magnetosheath, magnetopause, transition region and magnetotail current sheet. In particular, resolving ion composition in 3D is needed since energization mechanisms work differently for different ion species (e.g. heavy ion effects on reconnection rate). The Ion Mass Composition Analyser (IMCA) will be able to provide the three-dimensional (3D) distribution functions for the near-Earth main ion species (H+, He++ and O+) with an energy range covering the thermal and suprathermal energies and an energy and angular resolution permitting to study the non-Maxwellian features in the ions distribution functions. IMCA will be embarked on at least four of the seven Sister SpaceCraft (one SSC of the inner tetrahedron and the three outer SSCs) in order to provide mass resolved 3D distribution at the fluid scales. Embarking IMCA on all the seven SSCs is currently under consideration. Here we will report on the IMCA objectives, design and consortium.

How to cite: Marcucci, M. F. and the The Plasma Observatory IMCA Team: The Plasma Observatory Ion and Mass Composition Analyzer [IMCA], EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10626, https://doi.org/10.5194/egusphere-egu26-10626, 2026.

EGU26-10866 | ECS | Orals | ST2.2

Heat-flux instabilities of regularized Kappa distributed strahl electrons resolved with ALPS 

Dustin Lee Schröder, Marian Lazar, Rodrigo A. López, and Horst Fichtner

The fluid behavior of the solar wind is affected by the heat flux carried by the suprathermal electron populations, especially the electron strahl (or beam) that propagates along the magnetic field. 
In turn, the electron strahl cannot be stable, and in the absence of collisions, its properties are regulated mainly by self-generated instabilities.
This paper approaches the description of these heat-flux instabilities in a novel manner using regularized Kappa distributions (RKDs) to characterize the electron strahl. 
RKDs conform to the velocity distributions with suprathermal tails observed in-situ, and at the same time allow for consistent macromodeling, based on their singularity-free moments.
In contrast, the complexity of RKD models makes the analytical kinetic formalism complicated and still inaccessible, and therefore, here heat-flux instabilities are resolved using the advanced solver ALPS. 
Two primary types of instabilities emerge depending on plasma conditions: the whistler and firehose heat-flux instabilities.
The solver is successfully tested for the first time for such instabilities by comparison with previous results for standard distributions, such as Maxwellian and Kappa.
Moreover, the new RKD results show that idealized Maxwellian models can overrate or underestimate the effects of these instabilities, and also show differences from those obtained for the standard Kappa, which, for instance, underestimate the firehose heat-flux growth rates.

How to cite: Schröder, D. L., Lazar, M., López, R. A., and Fichtner, H.: Heat-flux instabilities of regularized Kappa distributed strahl electrons resolved with ALPS, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10866, https://doi.org/10.5194/egusphere-egu26-10866, 2026.

EGU26-10898 | Posters on site | ST2.2

Rado imaging of the interaction bewteen an coronal mass ejection  and nearby coronal structures 

Lei Lu, Li Feng, Jingye Yan, Xin Cheng, Yang Su, and Li Deng

Type II solar radio bursts are key tracers of shock waves driven by coronal mass ejections (CMEs), but identifying the precise location of the radio emission source along the extended shock front remains a major challenge. In the presented work, we investigate the origin of two successive, multi-lane metric Type II bursts observed on 16 February 2024. We utilize the novel radio imaging capabilities of the DAocheng Solar Radio Telescope (DART) in conjunction with white-light and EUV coronal observations from the Advanced Space-based Solar Observatory (ASO-S) and the Solar Dynamics Observatory (SDO). The initial Type II burst is imaged ahead of the erupting hot flux rope that develops into the CME. As the CME expands, a second, stronger Type II burst with two distinct emission lanes is detected. Our radio imaging analysis with DART unambiguously pinpoints the sources of these two lanes to the northern and southern flanks of the CME. Crucially, these sources correspond spatially and temporally to the interaction regions between the CME-driven shock and adjacent, dense coronal streamers. The significant enhancement of the radio emission at these locations provides direct evidence that shock-streamer interactions amplify the efficiency of particle acceleration. These observations demonstrate that different lanes in a multi-lane burst can originate from physically distinct regions along a non-uniform, rippled shock front, offering vital constraints on theories of particle energization in the solar corona and inner heliosphere.

 

How to cite: Lu, L., Feng, L., Yan, J., Cheng, X., Su, Y., and Deng, L.: Rado imaging of the interaction bewteen an coronal mass ejection  and nearby coronal structures, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10898, https://doi.org/10.5194/egusphere-egu26-10898, 2026.

EGU26-10927 | Posters on site | ST2.2

Improvements, extension and perspectives of the Cluster GRMB (Geospace Region and Magnetospheric Boundary identification) dataset 

Benjamin Grison, Matthew Taylor, Fabien Darrouzet, Romain Maggiolo, and Mychajlo Hajos

The purpose of the Geospace Region and Magnetospheric Boundary identification (GRMB) dataset is to provide information on the regions crossed by each of the 4 Cluster spacecraft during the entire mission. The dataset includes 15 labels, among which are: plasmasphere, plasmapause transition region (TR), plasmasheet TR, plasmasheet, lobes, polar regions, magnetopause TR, magnetopause, magnetosheath, bow shock TR, and solar wind and foreshock. The 4 remaining labels are: inside the magnetosphere, outside the magnetosphere, unknown, and no available data. This dataset has been delivered in 2024 to the Cluster Science Archive (CSA) covering the years 2001-2022: https://doi.org/10.57780/esa-85c563c.

We present updates and improvements made since this delivery. First, the available dataset publicly available at the CSA has been extended to the year 2023 and it will be extended to the end of the Cluster scientific mission (30 September 2024) by the end of 2026.

Second, a methodology update is addressing 2 aspects of the original dataset. The first one concerns IN/PLS and IN/PPTR labels following the update of the distance plots for C2, C3 and C4 completed during the first phase of the project. The second one concerns the descriptions of following inside labels: IN/PLS, IN/PPTR, IN/PSTR, IN/PSH, IN/LOB, and IN/POL to reduce the number of observations that could match 2 or more label definitions in the original methodology. The updated methodology is compatible with the original one, meaning that the updated dataset is more homogeneous. The outcome of these updates is illustrated with the years 2001-2002, which are reprocessed and delivered to the CSA in February 2026. Years 2001 to 2005 are not reprocessed to get a more precise dataset during the first years of the mission, when data availability and quality are the highest. This reprocessing shall be completed by the end of 2026.

Another important output of this dataset is to highlight the importance to identify the spacecraft location in term of Geospace environments. We therefore also discuss the possibility for the space plasma scientific community to have a normalized definition of the regions to ease multi-missions studies.

How to cite: Grison, B., Taylor, M., Darrouzet, F., Maggiolo, R., and Hajos, M.: Improvements, extension and perspectives of the Cluster GRMB (Geospace Region and Magnetospheric Boundary identification) dataset, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10927, https://doi.org/10.5194/egusphere-egu26-10927, 2026.

EGU26-11936 | Posters on site | ST2.2

Multi-scale intermittency and energy transfer in the terrestrial foreshock 

Peter Kovacs and Akos Madar

We investigate the space–time variability of intermittent magnetic turbulence in the terrestrial foreshock using fluxgate magnetometer observations from the Magnetospheric Multiscale (MMS) mission. Intermittency is quantified through sliding-window probability density function analysis and scale-dependent flatness of temporal magnetic field increments, over a broad range (0.2–256 s) of scales. The analysis is complemented by spectral diagnostics of the magnetic time-series. By organizing the analysis in terms of the field-aligned distance from the bow shock and the angle between the interplanetary magnetic field and the shock normal, we resolve systematic differences between quasi-parallel and quasi-perpendicular foreshock regions. The multi-spacecraft character of MMS enables us to directly probe spatial intermittency at the scale of the inter-spacecraft separations (~20 km), and compare spatial and temporal statistics, providing insight into the applicability of the Taylor hypothesis in a highly dynamic foreshock environment. We find that intermittency persists both below and beyond ion temporal scales, with enhanced intermittency in the quasi-parallel foreshock at sub-second scales and a reversal of this trend at larger scales. The latter finding is likely resulted in by intense wave activity. We emphasize that the provisional Plasma Observatory mission would enable our analyses to be extended to a broader range of spatial scales, providing a decisive advance in disentangling spatial and temporal variability and in understanding energy transfer in collisionless space plasmas.

Our study is conducted in the framework of the ESA-supported SWIFT project, which aims to investigate how solar wind dynamics drive turbulence and large-scale current structures within the coupled terrestrial magnetosphere–ionosphere system.

How to cite: Kovacs, P. and Madar, A.: Multi-scale intermittency and energy transfer in the terrestrial foreshock, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11936, https://doi.org/10.5194/egusphere-egu26-11936, 2026.

EGU26-12241 | Posters on site | ST2.2

The SCM instrument for the ESA Plasma Observatory mission 

Olivier Le Contel, Matthieu Kretzschmar, Alessandro Retino, Johann Gironnet, Guillaume Jannet, Fatima Mehrez, Dominique Alison, Claire Revillet, Laurent Mirioni, Clémence Agrapart, Nicolas Geyskens, Christophe Berthod, Gérard Sou, Thomas Chust, Clara Froment, Matthieu Berthomier, Cécile Fiachetti, Yuri Khotyaintsev, Vicki Crips, 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? After the Mission Consolidation Review by ESA in February 2025 followed by reformulation discussions, the mission now consists of seven identical small satellites (Sister spacecraft, SSC) equipped by an updated payload, still 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. 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 now required on the seven SSC. SCM will be delivered by LPP and LPC2E and will provide the three components of the magnetic field fluctuations in the [1Hz-8kHz] frequency range, after digitization by the wave analyser board (WAB) within the electric and magnetic electronics box (BOX-W), relevant for the three key science regions. Continuous waveforms and snapshots every 4 s, will be sampled at 512 Hz and 16 kHz respectively. SCM is planned to be mounted on a 1.5-2 m boom and will have the following sensitivity performances [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) of the WAVES instrument suite, 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 and partitioning processes, the plasma and energy transport, the acceleration and the heating of the plasma.

How to cite: Le Contel, O., Kretzschmar, M., Retino, A., Gironnet, J., Jannet, G., Mehrez, F., Alison, D., Revillet, C., Mirioni, L., Agrapart, C., Geyskens, N., Berthod, C., Sou, G., Chust, T., Froment, C., Berthomier, M., Fiachetti, C., Khotyaintsev, Y., Crips, V., and Marcucci, M. F.: The SCM instrument for the ESA Plasma Observatory mission, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12241, https://doi.org/10.5194/egusphere-egu26-12241, 2026.

EGU26-12594 | Orals | ST2.2

Multi-scale processes at the transition region of the Earth’s magnetotail 

Rumi Nakamura, Evgeny Panov, Martin Hosner, Markku Alho, Lauri Pänkäläinen, and Alessandro Retino

The interaction between localized fast plasma jets, called bursty bulk flows (BBF) or flow bursts and ambient magnetic field plays an important role in the complex chain of solar wind-magnetosphere-ionosphere coupling processes.  In particular the transition region, where the magnetic field configuration changes from dipolar-like configuration to tail-like configuration and where near-Earth flow braking/bouncing processes take place, is a key region of fundamental processes such as the particle energization and wave-particle interaction. These processes, associated with magnetic and pressure disturbances, drive enhanced energy and momentum transfer from the nightside outer magnetosphere along Earth’s magnetic field lines down to the ionosphere. Across the field lines, particle injections further affect the inner magnetosphere dynamics, constituting a source population for the radiation belt and the ring current.

In this presentation we stress the importance of observations of BBFs and dipolarization fronts by multi-point measurements in an extensive region covering both equatorial and off-equatorial  locations, and simultaneously at ion and fluid scales for understanding the energy transport processes. These allows us to monitor both the field-aligned and perpendicular evolution of the flux tube and enable to study the coupling with the ionosphere.  By showing several examples of observations from previous studies of different scales of disturbances and fortuitous multi-spacecraft configuration at different scales, the 3D nature of the interaction between the BBF and ambient plasma, and its relationship to ionosphere including field-aligned current and aurora will be discussed.

 

How to cite: Nakamura, R., Panov, E., Hosner, M., Alho, M., Pänkäläinen, L., and Retino, A.: Multi-scale processes at the transition region of the Earth’s magnetotail, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12594, https://doi.org/10.5194/egusphere-egu26-12594, 2026.

EGU26-12667 | Posters on site | ST2.2

Are the tearing and the Weibel instabilities the same? 

Kevin Schoeffler, Harikrishnan Aravindakshan, and Maria Elena Innocenti

The tearing instability, which takes free energy from oppositely directed magnetic fields, and the Weibel instability, which takes free energy from temperature anisotropies, at first glance, appear to be entirely different instabilities. However, the opposing magnetic fields enforce a current between them, and the associated drift of the plasma leads to an effective thermal spread that is larger along the direction of the flow. This modified thermal spread acts as a temperature anisotropy that helps drive the instability. We investigate the connection between the two instabilities using 2D semi-implicit particle-in-cell simulations (with the code ECSIM), starting from a Harris equilibrium and no guide field. We find that for thin current sheets (thinner than the ion Larmor radius), where the assumptions of the kinetic tearing instability from Zelenyi & Krasnosel'skikh (1979) break down, the Weibel theory gives a better estimate for the growth of the instability.

How to cite: Schoeffler, K., Aravindakshan, H., and Innocenti, M. E.: Are the tearing and the Weibel instabilities the same?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12667, https://doi.org/10.5194/egusphere-egu26-12667, 2026.

EGU26-12854 | Posters on site | ST2.2

Waves instrument suite for the ESA Plasma Observatory mission 

Yuri Khotyaintsev, Olivier Le Contel, Matthieu Kretzschmar, Marek Morawski, Cecilia Norgren, Jan Soucek, Vicki Cripps, Walter Puccio, Gabriel Giono, Fabrice Colin, Guillaume Jannet, Konrad Aleksiejuk, Paweł Szewczyk, and Hanna Rothkaehl

The Waves instrument suite for the ESA Plasma Observatory mission provides coordinated measurements of electromagnetic fields in space plasmas to address key phenomena affecting particle energization, including plasma waves, turbulence, and wave-particle interactions. The suite consists of an Electric Field Instrument (EFI) and a Search Coil Magnetometer (SCM), enabling simultaneous observations of electric and magnetic field fluctuations and the spacecraft potential. Both electric and magnetic sensors are connected to a common electronics unit, BOX-W, which performs synchronized sampling and on-board processing. BOX-W supports both waveform capture and spectral products, enabling efficient use of telemetry while retaining scientifically relevant information. The combined EFI and SCM measurements enable full characterization of electromagnetic fluctuations, facilitating the determination of wave polarization, propagation properties, and energy flux.

How to cite: Khotyaintsev, Y., Le Contel, O., Kretzschmar, M., Morawski, M., Norgren, C., Soucek, J., Cripps, V., Puccio, W., Giono, G., Colin, F., Jannet, G., Aleksiejuk, K., Szewczyk, P., and Rothkaehl, H.: Waves instrument suite for the ESA Plasma Observatory mission, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12854, https://doi.org/10.5194/egusphere-egu26-12854, 2026.

EGU26-12905 | Posters on site | ST2.2

Cessation and restart of reconnection -- observations from the exhaust 

Cecilia Norgren, Michael Hesse, Tai Phan, Yuri Khotyaintsev, and Louis Richard

Magnetic reconnection in Earth’s magnetotail is inherently intermittent, yet the physical processes governing its cessation and subsequent restart remain poorly understood, largely due to the multiscale nature of the system. In this study, we use high-resolution, multi-point observations from the Magnetospheric Multiscale (MMS) mission to investigate a three-phase event from the terrestrial magnetotail in which reconnection is initially active, subsequently absent for several minutes, and then reinitiates.

The event begins with an off-equatorial, field-aligned ion jet indicative of ongoing reconnection. This jet is replaced by a prolonged quiet interval characterized by a duskward ion flow carried by a hot population, negligible ExB drift, and the absence of conventional reconnection signatures. During this interval, the total plasma plus magnetic pressure increases, and the observations reveal evidence for current sheet thickening followed by thinning. 

The first indication of renewed activity is an injection of energetic field-aligned ions detected off-equatorially, followed by the gradual formation of an equatorial plasma jet and the subsequent arrival of dipolarization fronts. The first dipolarization front clearly separates ions originating from the pre-existing plasma sheet and the lobes, signalling the arrival of magnetic flux tubes that were among the first to reconnect during onset. At the onset of the emerging jet, prior to the arrival of the first dipolarization front, ions briefly become demagnetized and a northward electric field is observed, opposite in sign to the typical Hall electric field expected in the ion diffusion region. These signatures highlight the complex and transient nature of the plasma environment during the evolution of a reconnection outflow jet and point to processes that cannot be fully resolved with the MMS tetrahedron alone.

These observations demonstrate that to understand reconnection intermittency requires simultaneous measurements spanning electron, ion, and magnetohydrodynamic scales. Plasma Observatory, providing coordinated multi-point coverage across these scales, is essential for capturing the coupled evolution of particles, fields, and currents during reconnection cessation and onset—processes that cannot be resolved with present-day multi-spacecraft constellations.

How to cite: Norgren, C., Hesse, M., Phan, T., Khotyaintsev, Y., and Richard, L.: Cessation and restart of reconnection -- observations from the exhaust, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12905, https://doi.org/10.5194/egusphere-egu26-12905, 2026.

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 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, as well as for the comprehension of distant astrophysical plasma environments. In situ observations, theory and simulations suggest that the largest amount of  plasma energization and energy transport occur through the coupling between large, fluid scales and the smaller, ion kinetic scales. Remote observations currently cannot access these scales, and existing multi-point in situ observations do not have a sufficient number of observation points to resolve the fluid-ion scale coupling. 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 in key regions where the strongest plasma energization and energy transport occur: 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 address the two Plasma Observatory Science Objectives (SO1) How are particles energized in space plasmas? and (SO2) 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 in the Solar System and of distant astrophysical plasmas. 

How to cite: Retinò, A. and Marcucci, M. F. and the Plasma Observatory Team: Unveiling plasma energization and energy transport in the Magnetospheric System through multi-scale observations: the science of the ESA M7 Plasma Observatory mission candidate, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13019, https://doi.org/10.5194/egusphere-egu26-13019, 2026.

EGU26-13407 | Orals | ST2.2

Validation of Landau-Fluid Closures for Kinetic-Scale Plasma Turbulence: A Comparison with Fully Kinetic Simulations  

Simon Lautenbach, Jeremiah Lübke, Maria Elena Innocenti, Katharina Kormann, and Rainer Grauer

Understanding energy cascades across multiple scales remains challenging in magnetospheric physics, where processes span from large fluid scales down to kinetic scales. Two-fluid simulations employing local Landau-fluid closures offer a computationally efficient alternative to kinetic simulations for modeling the multiscale plasma dynamics. These closures, derived from linear kinetic theory, approximate kinetic effects while maintaining the computational advantages of fluid descriptions. However, their theoretical validity requires the plasma to remain close to local thermodynamic equilibrium (LTE), a condition frequently violated in magnetospheric phenomena such as turbulence in the magnetosheath and reconnection outflows.

We investigate the performance of two-fluid Landau-fluid models in regimes far from LTE through comparison against benchmark Vlasov simulations. Our results demonstrate that despite operating outside their formal regime of applicability, Landau-fluid closures can accurately reproduce kinetic-scale physics (with some limitations that we will highlight) when the local closure parameter is appropriately chosen. The agreement of energy spectra extends across the kinetic range, capturing the essential energy cascade and dissipation mechanisms.

These findings validate Landau-fluid approaches as a robust tool for large-scale magnetospheric simulations where computational constraints prohibit kinetic treatments. This is particularly relevant for interpreting multiscale observations and resolve scale coupling in key magnetospheric regions. 

How to cite: Lautenbach, S., Lübke, J., Innocenti, M. E., Kormann, K., and Grauer, R.: Validation of Landau-Fluid Closures for Kinetic-Scale Plasma Turbulence: A Comparison with Fully Kinetic Simulations , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13407, https://doi.org/10.5194/egusphere-egu26-13407, 2026.

EGU26-13489 | Orals | ST2.2 | Highlight

The ESA M7 candidate mission Plasma Observatory: unveiling plasma energization and energy transport in the Magnetospheric System with multiscale observations 

Maria Federica Marcucci and Alessandro Retinò and the Plasma Observatory Team

Plasma energization and transport of energy are key open problems of space plasma physics. Their comprehension is a grand challenge of plasma physics that has implications on research fields that span from space weather to the understanding of the farthest astrophysical plasmas. The Earth’s Magnetospheric System is a  complex and highly dynamic plasma environment where strong energization and energy transport occurs and it is the best natural laboratory to study these processes through in situ measurements. Theory, numerical simulations and previous multi-point observations from missions such as ESA/Cluster and NASA/MMS evidenced that cross-scale coupling has a fundamental role in plasma energization and energy transport. Therefore, in order to ultimately understand these key processes, simultaneous in situ measurements at both large, fluid and small, kinetic scales are required. Such measurements are currently not available. 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 simultaneous measurements at both fluid and ion scales. These are the scales at which the largest amount of electromagnetic energy is converted into energized particles and energy is transported. PO has an HEO 7.2x17 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 magnetotail current sheet. PO baseline mission includes seven identical smallsat Sister Space Craft (SSC) in two nested tetrahedra formation. The tetrahedra separation scales cover all typical ion and fluid scales of interest in the Key Science Regions  and vary between about 50 km and 5000 km. The SSC payload provides a complete characterization of electromagnetic fields and particles simultaneously at multiple locations with measurements tailored to ion and fluid scales. 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 June 2026 and launch in 2037.

How to cite: Marcucci, M. F. and Retinò, A. and the Plasma Observatory Team: The ESA M7 candidate mission Plasma Observatory: unveiling plasma energization and energy transport in the Magnetospheric System with multiscale observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13489, https://doi.org/10.5194/egusphere-egu26-13489, 2026.

EGU26-14170 | ECS | Posters on site | ST2.2

How do electrons shape the proton distribution functions near the Sun? 

Mahmoud Saad Afify Ali Ibrahim, Jürgen Dreher, Kristopher G. Klein, Stuart O'Neill, Mihailo M. Martinović, and Maria Elena Innocenti

Observations from the Parker Solar Probe (PSP) reveal that electrons play a crucial role in shaping coronal and solar wind dynamics (Halekas et al. 2021, 2022, 2025). We investigate how nonthermal ( κ ) and core/strahl electron distributions modify the onset threshold of the ion-ion acoustic instability (IIAI) observed by PSP between 15-25 solar radii (Mozer et al. 2021, 2023; Kellogg et al. 2024) and modeled by Afify et al. (2024). We find that (Afify et al. 2025):

  • lower κ values tend to stabilize IIAI due to higher electron phase space density at the resonance velocity, which leads to enhanced Landau damping in the electrons;
  • the presence of a strahl population shifts the resonance velocity with respect to that obtained with the core distribution alone, thus modifying the IIAI threshold. An effective temperature can be calculated from core and strahl parameters (Jones et al. 1975), which allows to map the core-strahl system to one with a single electron population and simplify threshold and growth rate calculations;
  • Applying the field-particle correlation technique (Klein & Howes 2016) to fully kinetic Vlasov simulations reveals detailed velocity-space energy transfer in the presence of the different electron distributions (Afify et al. 2026) and indicates that Landau damping plays a significant role in reducing free energy and contributing to heating.

Future work will address the interplay between electron and ion anisotropies in low-β regimes.

References

Afify, M. A., Dreher, J., Schoeffler, K., Micera, A., & Innocenti, M. E. 2024, APJ, 971, 93
Afify, M. S., Dreher, J., O'Neill, S., & Innocenti, M. E. 2025, A&A, 702, A277
Afify, M. S., Klein, K. G., Martinović, M. M., & Innocenti, M. E. 2026, arXiv:2601.08329.
Halekas, J., Berčič, L., Whittlesey, P., et al. 2021, ApJ, 916, 16.
Halekas, J., Whittlesey, P., Larson, D., et al. 2022, ApJ, 936, 53.
Halekas, J., Whittlesey, P., Larson, D., et al. 2025, ApJ, 993, 19., 993, 19
Jones, W., Lee, A., Gleman, S., & Doucet, H. 1975, Physical Review Letters, 35, 1349
Kellogg, P. J., Mozer, F. S., Moncuquet, M., et al. 2024, ApJ 964, 68.
Klein, K. G. & Howes, G. G. 2016, APJL, 826, L30
Mozer, F., Bale, S., Kellogg, P., et al. 2023, Phys. Plasmas, 062111, 30
Mozer, F. S., Vasko, I. Y., & Verniero, J. L. 2021, ApJL, 919, L2.

How to cite: Ibrahim, M. S. A. A., Dreher, J., Klein, K. G., O'Neill, S., Martinović, M. M., and Innocenti, M. E.: How do electrons shape the proton distribution functions near the Sun?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14170, https://doi.org/10.5194/egusphere-egu26-14170, 2026.

EGU26-15134 | Posters on site | ST2.2

Polish contribution to the PMO mission 

Hanna Rothkaehl, Marek Morawski, Konrad Aleksiejuk, Paweł Szewczyk, Grzegorz Ptasiński, Barabara Matyjasiak, Dorota Przepiórka Skup, and Tomasz Barciński

The general idea  for   instruments arcitecture for the PMO  mission is to have the identical  set of instruments located on the board of seven identical spacecraft,  via  the  two independent interface connections to the spacecraft managed by two electronic boxes: BOX-W and BOX-P

The Polish contribution to the PMO mission includes scientific,  instruments and management aspects for both BOX-P and BOX-W units.  CBK PAS leads the activity in the frame of BOX-P at management and system engineering.

The BOX-P instrument serves as a common electronics box, housing the front-end electronics for the flux gate magnetometer MAG and its sensors, a common power supply unit PSU, and a common Data Processing Unit DPU. The BOX-P electronics box also implements the common power and

data interface for the particle diagnostics instruments: iEPC, EPE and IMCA. BOX-P implements the single communication interface for the entire sisters spacecraft payload. All sets of instruments are dedicated to the in situ, multi-scale, multi-point study, through simultaneous measurements, of plasma energisation and energy transport in the Earth's Magnetospheric System.

CBK PAS  leads  the activity for EFI, the Electric Field Antenna and the manufacturing EFI-ADA sensor.  The Electric Field Dipole Antenna (EFI-ADA) is connected to the BOX-W suit instrument, which measures the AC electric field from DC to 100 kHz. The EFI-ADA sensor consists of a single dipole antenna. The sensor will be mounted near the end of the rigid magnetometer boom on which SCM is mounted and will feature an orthogonal-to-the-boom dipole antenna, approximately 4.0 meters from tip to tip.

CBK PAS will also design and manufacture the power supply unit, PSU unit for BOX-W .     

 

 

How to cite: Rothkaehl, H., Morawski, M., Aleksiejuk, K., Szewczyk, P., Ptasiński, G., Matyjasiak, B., Przepiórka Skup, D., and Barciński, T.: Polish contribution to the PMO mission, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15134, https://doi.org/10.5194/egusphere-egu26-15134, 2026.

EGU26-15373 | Orals | ST2.2

Rigorous Calculation of the Energy Release in Solar Eruptions with the SCEPTER Model 

Spiro Antiochos, Bart Van Der Holst, Nishtha Sachdeva, Gabor Toth, Joel Dahlin, Tamas Gombosi, and Judit Szente

Magnetic reconnection in coronal current sheet(s) is widely believed to be the main energy release process powering solar eruptive events, such as flares, coronal mass ejections (CME), and coronal jets. Modeling this process and determining the channels for the energy release, mass motions and heating, has long been a major goal in space science. We present results from a two-fluid MHD simulation of an eruptive flare/CME using a newly developed Strategic Capability, SCEPTER, which is based on the well-validated and widely used Space Weather Modeling Framework. SCEPTER incorporates two major advances in numerical capability. First, we use the STITCH formalism for the energy buildup, so that we start with a potential-field minimum-energy state and slowly form a sheared filament channel over a polarity inversion line as is observed on the Sun. Second, we use a new formulation of the plasma energetics that is explicitly energy conserving while calculating separate electron and ion temperatures and separate parallel and perpendicular pressures, as desired. For this first simulation with our new model, we opted for the non-adiabatic heating to go solely into the protons and for an isotropic pressure. We discuss the resulting energetics of the reconnection and, in particular, the plasma heating in the reconnecting current sheets, mass acceleration, and shock formation. We also discuss the implications of our results for understanding solar eruptions, in general.

 

This work was supported by the NASA Living With a Star Program.

 

How to cite: Antiochos, S., Van Der Holst, B., Sachdeva, N., Toth, G., Dahlin, J., Gombosi, T., and Szente, J.: Rigorous Calculation of the Energy Release in Solar Eruptions with the SCEPTER Model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15373, https://doi.org/10.5194/egusphere-egu26-15373, 2026.

EGU26-15442 | Posters on site | ST2.2

The Energetic Particle Experiment on Plasma Observatory 

Vassilis Angelopoulos, Malcolm Dunlop, Rami Vainio, Robert Wimmer-Schweingruber, Demet Ulusen Aksoy, Ethan Tsai, Mark Prydderch, Lars Berger, Christopher Liu, Ryan Caron, Jussi Lehti, Alex Steven, William Grainger, Nicole Melzack, Murali Nalagatla, Svea Jürgensen, Patrick Kühl, Hannes Ebeling, and Colin Wilkins

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 seven sister 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 Experiment (EPE). Here we present the instrument, which is a compact, dual-particle telescope, solid state detector design originally based on ELFIN’s EPD instrument. Using three telescopes (sensor heads), 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 Aluminized Kapton foil covers to screen out low energy ions on electron side. The baseline energy range (30-600 keV) for both species (with a goal for 20-600 keV at spin cadence) is targeted on low-end, suprathermal energies (minimising the effective gyro-scales for the computation of moments, PAD (e) and VDF determination). An extended energy range of up to 1.5 MeV at lower cadence is possible for ions.  This arrangement allows the potential for spatial differences to be resolved on at least ion to fluid scales and to sense plasma boundaries. Detector layering is based on expected dynamic energy range and allows coincident/anti-coincident logic to be applied to separate out the higher energy species.

How to cite: Angelopoulos, V., Dunlop, M., Vainio, R., Wimmer-Schweingruber, R., Ulusen Aksoy, D., Tsai, E., Prydderch, M., Berger, L., Liu, C., Caron, R., Lehti, J., Steven, A., Grainger, W., Melzack, N., Nalagatla, M., Jürgensen, S., Kühl, P., Ebeling, H., and Wilkins, C.: The Energetic Particle Experiment on Plasma Observatory, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15442, https://doi.org/10.5194/egusphere-egu26-15442, 2026.

EGU26-15945 | Posters on site | ST2.2

Development of a Time of Flight section for a Mass Spectrometer for the future Plasma Observatory mission. 

Harald Kucharek, Lynn Kistler, Christoforos Mouikis, Elisabetta De Angelis, Yvon Alata, Markus Fraenz, Fedeica Marcucci, Alessandro Retino, and Alessandro Brin

In this presentation we report on the development of an Ion mass instrument onboard of small Sat as part of the Plasma Observatory mission. This new Ion Mass Spectrometer that will be developed for this mission is similar to the IES-D instrument successfully flown on the Cluster II mission. The IMS instrument developed for the THOR mission. The TOF (Time of Flight) section is similar but smaller than designed for the THOR mission. That clearly indicates a high level of heritage of this Mass Spectrometer. Hence this IMCA like instrument for Plasma Observatory this is a new instrument that will have a smaller TOF chamber we have redesigned the TOF section by using SIMION and TRIM simulations to evaluate the performance/geometric factor of this new instrument and the effect of thin carbon foils. The first results of this study indicated that we will be able to measure Hydrogen, Helium and Oxygen ions with sufficient high statistic in all science areas of this mission. covering the thermal and suprathermal energies, with a time resolution enabling to resolve ion scales and an energy and angular resolution permitting to study the non-Maxwellian features in distribution functions. Thus, the energy range will be 10eV - 30keV with a 20% resolution, a temporal resolution: 2s and an angular resolution: 22.5°. It is also planned to add a flux reducer to this sensor the handle a large dynamic range. In this presentation we will report on the current status of this development.

How to cite: Kucharek, H., Kistler, L., Mouikis, C., De Angelis, E., Alata, Y., Fraenz, M., Marcucci, F., Retino, A., and Brin, A.: Development of a Time of Flight section for a Mass Spectrometer for the future Plasma Observatory mission., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15945, https://doi.org/10.5194/egusphere-egu26-15945, 2026.

High-energy charged particles are ubiquitous in astrophysical, space, and laboratory plasmas, and identifying underlying acceleration mechanisms remains a fundamental challenge. In Earth’s magnetotail, it has been proposed that particles in the mid-magnetotail are initially accelerated to tens to hundreds of keV by magnetic reconnection and subsequently transported to the near-Earth magnetotail, where they are further energized to MeV energies via wave–particle interactions. However, this paradigm hasn’t been verified and particle acceleration processes remain highly controversial. Here, we identify a previously unrecognized acceleration mechanism, dubbed Magnetic Rayleigh–Taylor (MRT) instability, which produces high energy particles up to ~1MeV in the magnetotail. Once the instability is triggered, numerous instability heads characterized by sharp magnetic field enhancements with surrounding flow vortices are generated. As these heads propagate earthward, electron Kelvin–Helmholtz (KH) instabilities are excited and generate super-intense localized electric fields that efficiently accelerates both electrons and ions trapped within the heads. This process results in electron power-law energy spectra with progressively harder indices closer to Earth. These findings demonstrate that the MRT instability is an efficient particle acceleration mechanism in the magnetotail and may significantly contribute to the high-energy particle populations in Earth’s outer radiation belt.

How to cite: Wang, R.: Particle acceleration by Magnetic Rayleigh–Taylor instability in the near-Earth magnetotail, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16676, https://doi.org/10.5194/egusphere-egu26-16676, 2026.

EGU26-17034 | Posters on site | ST2.2

Modelling magnetic helicity flux through solar photosphere from ASO-S/FMG 

Shangbin Yang, Suo Liu, Jiangtao Su, and Yuanyong Deng

Magnetic helicity is a key geometrical parameter to describe the structure and evolution of
solar coronal magnetic fields. The accumulation of magnetic helicity is correlated with the
nonpotential magnetic field energy, which is released in the solar eruptions. Moreover, the
relative magnetic helicity fluxes can be estimated only relying on the line-of-sight magnetic
field (e.g. Démoulin and Berger 2003). The payload Full-disk MagnetoGraph (FMG) on the
Advanced Space-based Solar Observatory (ASO-S) currently has been supplying the con-
tinuous evolution of line-of-sight magnetograms for the solar active regions, which can be
used to estimate the magnetic helicity flux. In this study, we use eight-hour line-of-sight
magnetograms of NOAA 13273, at which the Sun–Earth direction speed of the satellite is
zero to avoid the oscillation of the magnetic field caused by the Doppler effect on polar-
ization measurements. We obtain the helicity flux by applying fast Fourier transform (FFT)
and local correlation tracking (LCT) methods to obtain the horizontal vector potential field
and the motions of the line-of-sight polarities. We also compare the helicity flux derived
using data from the Heliosesmic and Magnetic Imager (HMI) on board the Solar Dynamics
Observatory (SDO) and the same method. It is found that the flux has the same sign and the
correlation between measurements is 0.98. The difference of the absolute magnetic helicity
normalized to the magnetic flux is less than 4%. This comparison demonstrates the reliabil-
ity of ASO-S/FMG data and that it can be reliably used in future studies.

How to cite: Yang, S., Liu, S., Su, J., and Deng, Y.: Modelling magnetic helicity flux through solar photosphere from ASO-S/FMG, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17034, https://doi.org/10.5194/egusphere-egu26-17034, 2026.

EGU26-17097 | Orals | ST2.2

Turbulence-Driven Magnetic Reconnection: From Cluster and Magnetospheric Multiscale to Plasma Observatory 

Julia E. Stawarz, Luca Franci, Paulina Quijia Pilapaña, Jeffersson Agudelo Rueda, Prayash S. Pyakurel, Michael A. Shay, Tai D. Phan, Naoki Bessho, and Imogen L. Gingell

Magnetic reconnection events generated by tangled magnetic fields produced in turbulent plasmas have long been thought to play an important role in turbulent dynamics. These events have traditionally been challenging to examine from either a numerical or observational perspective due to their small-scale nature and complex magnetic topologies. However, multi-spacecraft measurements have provided a step-change in understanding this complex phenomenon. Since the days of Cluster, evidence has been found for turbulence-driven magnetic reconnection embedded within the turbulent fluctuations of Earth's magnetosheath, making it an ideal location for studying the physics and importance of turbulence-driven magnetic reconnection. In this presentation, we will highlight the observational insights into turbulence-driven reconnection that have been enabled by the systematic identification and analysis of reconnection events in Earth's magnetosheath by missions such as NASA's Magnetospheric Multiscale (MMS) and ESA’s Cluster missions – including the importance of so-called electron-only reconnection and estimates that suggest magnetic reconnection can account for a significant fraction of the energy dissipated in turbulent plasmas. Using kinetic simulations of turbulence reminiscent of the plasmas found in Earth’s magnetosheath, we will further demonstrate and evaluate how multi-scale measurements from a mission such as ESA’s proposed Plasma Observatory will enable key observational constraints characterizing the 3D structure and distribution of turbulence-driven magnetic reconnection events that will usher in a new era of advancements on the subject.

How to cite: Stawarz, J. E., Franci, L., Quijia Pilapaña, P., Agudelo Rueda, J., Pyakurel, P. S., Shay, M. A., Phan, T. D., Bessho, N., and Gingell, I. L.: Turbulence-Driven Magnetic Reconnection: From Cluster and Magnetospheric Multiscale to Plasma Observatory, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17097, https://doi.org/10.5194/egusphere-egu26-17097, 2026.

EGU26-18602 | Posters on site | ST2.2

Interchange Reconnection and ion kinetic instabilities in coronal plasma 

Vladimir Krasnosselskikh, Arnaud . Zaslavsky, Pierre-Louis Sulem, Immanuel Christopher Jebaraj, Thierry Dudok de Wit, Jaye Verniero, Vadim Roytershteyn, Oleksiy Agapitov, and Michael Balikhin

The magnetic field in the chromosphere and low corona near the boundaries of equatorial coronal holes in the quiet Sun is thought to reconfigure through interchange reconnection (IR). This process occurs in low-beta plasma with a strong guiding field and may produce an ion distributions known as “hammerhead.”  These distributions have been observed in coronal plasma associated with current sheets and in regions whose footpoints lie near equatorial coronal holes. They usually consist of a core plus a perpendicularly diffuse beam feature at a specific velocity relative to the core. The mechanism we propose involves the interpenetration of two plasmas with different properties—one on closed field lines and one on open field lines. In the chromosphere and low corona, these distributions can generate ion-sound and ion-cyclotron waves once the beam’s relative velocity exceeds a threshold. As such plasma distributions travel toward the solar wind through a funnel region where the magnetic field and plasma density rapidly drop, they may become unstable and produce Alfvén-type magnetic perturbations that can evolve nonlinearly into switchback structures. These threshold conditions are likely met near the transition from sub-Alfvénic to super-Alfvénic wind.

How to cite: Krasnosselskikh, V., . Zaslavsky, A., Sulem, P.-L., Jebaraj, I. C., Dudok de Wit, T., Verniero, J., Roytershteyn, V., Agapitov, O., and Balikhin, M.: Interchange Reconnection and ion kinetic instabilities in coronal plasma, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18602, https://doi.org/10.5194/egusphere-egu26-18602, 2026.

EGU26-19090 | Orals | ST2.2

Multiscale Wave-Particle Interactions for Plasma Energization and Energy Transport: Open, Fundamental Questions that Plasma Observatory Can Solve 

Oliver Allanson, Clare Watt, Jonathan Rae, Adnane Osmane, Jean-Francois Ripoll, David Hartley, Miroslav Hanzelka, Anton Artemyev, Julia Stawarz, Daniel Ratliff, Ravindra Desai, Sarah Bentley, Colin Forsyth, Suman Chakraborty, Rachel Black, Samuel Hunter, Nigel Meredith, Xiaojia Zhang, and Leonid Olifer and the ISSI team 25-640: Beyond Diffusion - Advancing Earth’s Radiation Belt Models with Nonlinear Dynamics

Wave-particle interactions are a fundamental mechanism to control irreversible plasma energization and energy transport throughout the Heliosphere, and universally throughout astrophysical plasma domains. The most tractable paradigm to model the plasma response to perturbations by plasma waves is the 60 year old quasilinear diffusion theory. This paradigm predominates in our understanding, but within the last two decades there has been a sustained resurgence and emergence of fundamental new questions motivated by the discovery of highly variable, intense/energetic and structured electromagnetic plasma waves and wave-particle interaction plasma physics processes by single and multi-point missions. These interactions act and control plasma energization and energy transport from microscale (gyroradius/kinetic) through to the macroscale (system scale), and in addition crucially link these scales via complex coupled fluid/mesoscale plasma physics processes. We discuss recent advances, and highlight some open, fundamental questions for wave-particle interactions that the Plasma Observatory Mission can solve via multiscale observations.

How to cite: Allanson, O., Watt, C., Rae, J., Osmane, A., Ripoll, J.-F., Hartley, D., Hanzelka, M., Artemyev, A., Stawarz, J., Ratliff, D., Desai, R., Bentley, S., Forsyth, C., Chakraborty, S., Black, R., Hunter, S., Meredith, N., Zhang, X., and Olifer, L. and the ISSI team 25-640: Beyond Diffusion - Advancing Earth’s Radiation Belt Models with Nonlinear Dynamics: Multiscale Wave-Particle Interactions for Plasma Energization and Energy Transport: Open, Fundamental Questions that Plasma Observatory Can Solve, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19090, https://doi.org/10.5194/egusphere-egu26-19090, 2026.

EGU26-19230 | ECS | Posters on site | ST2.2

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 (PO) 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 2026, Vienna, Austria, 3–8 May 2026, EGU26-19230, https://doi.org/10.5194/egusphere-egu26-19230, 2026.

EGU26-19304 | ECS | Posters on site | ST2.2

The Plasma Observatory Synergies and Additional Science Working Group 

Simone Benella, Jean-Francois Ripoll, Cecilia Norgren, Oliver Allanson, Lorenzo Biasiotti, Sara Gasparini, Matina Gkioulidou, Stavro Lambrov Ivanovski, Hantao Ji, Barbara Matyjasiak, Yoshi Miyoshi, Rumi Nakamura, Alexander Pitna, Dorota Przepiórka-Skup, Virgilio Quattrociocchi, Adriana Settino, Marina Stepanova, Sergio Toledo-Redondo, Drew Turner, and Emiliya Yordanova

The main aim of the ESA Class-M7 Plasma Observatory (PO) mission currently in Phase A, is to explore the multiscale physics governing energy transfer and particle energization in near-Earth space plasmas. Flying a constellation of seven spacecraft in a double nested tetrahedral configuration, PO will deliver simultaneous measurements of fields, waves, and particles across ion, sub-ion, and MHD scales in various regions of the near-Earth space, within 7 to 13 Earth radii. While the mission core science focuses on regions such as the bow shock, magnetosheath, magnetopause, and plasma sheet, the orbital design naturally enables extensive coverage of additional regions, including the inner magnetosphere, the flanks of the magnetopause, and the ambient solar wind. The Synergies and Additional Science Working Group investigates the scientific opportunities enabled by PO observations beyond the primary science regions and aims to broaden the mission scientific impact through cross-disciplinary synergies. The solar-wind-driven magnetosphere is a highly dynamic system in which key processes can only be resolved through multipoint, multiscale observations.

With seven-point measurements, PO will allow the multiscale characterization of M-I coupling and plasma sources of both solar wind and ionospheric origin under varying geomagnetic conditions. In the inner magnetosphere, PO will address fundamental questions on wave propagation and wave-particle interactions at the edge of the outer radiation belt. Multipoint observations of ULF, EMIC, chorus, and whistler-mode waves will enable direct in-situ identification of acceleration, transport, and loss processes of energetic particles. PO will also resolve the multiscale structure and evolution of plasmaspheric plumes of cold plasma and assess their role in wave generation and radiation belt dynamics. At the flank magnetopause and in the upstream solar wind, PO will probe the coupling between large-scale plasma dynamics, turbulence, and kinetic dissipation. Simultaneous measurements at multiple scales will allow detailed investigations of Kelvin-Helmholtz instability, reconnection, plasma mixing, and turbulent energy transfer, as well as accessing the fine structure of solar wind transients that control mass and energy input into the magnetosphere.

PO will further enable strong synergies with other heliophysics missions, laboratory plasma experiments, and space weather research. PO multiscale observations will improve constraints on M-I coupling currents, geomagnetically induced currents, and CME-driven disturbances, while providing a unique space-based counterpart to laboratory reconnection experiments. This contribution summarizes recent progress within the Synergies and Additional Science Working Group and outlines future perspectives supporting PO during Phase A.

How to cite: Benella, S., Ripoll, J.-F., Norgren, C., Allanson, O., Biasiotti, L., Gasparini, S., Gkioulidou, M., Ivanovski, S. L., Ji, H., Matyjasiak, B., Miyoshi, Y., Nakamura, R., Pitna, A., Przepiórka-Skup, D., Quattrociocchi, V., Settino, A., Stepanova, M., Toledo-Redondo, S., Turner, D., and Yordanova, E.: The Plasma Observatory Synergies and Additional Science Working Group, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19304, https://doi.org/10.5194/egusphere-egu26-19304, 2026.

EGU26-19522 | ECS | Posters on site | ST2.2

Preliminary analyses of Surface Charging effects for the Plasma Observatory (PMO) mission 

Marianna Michelagnoli, Maria Federica Marcucci, Alessandro Retinò, Matthieu Berthomier, Yuri Khotyaintsev, Anders Eriksson, Jan Soucek, Fredrik Johansson, Fabrice Cipriani, Mauro Focardi, and Pierpaolo Merola

Plasma Observatory (PMO) 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 June 2026 and launch in 2037. PO scientific theme is unveiling plasma energization and energy transport in the near-Earth plasma environment through multiscale observations. The baseline mission includes seven identical smallsat Sister Space Craft (SSC) embarking state of the art instruments for electromagnetic fields and particle measurements. This work presents the results of preliminary surface charging analyses performed for the PMO.

Surface charging phenomenon is induced by the interaction of the spacecraft with the surrounding plasma environment and can lead to several potentially harmful consequences, including interference with ground communications, on-board electronics and scientific instruments. Since PMO aims to investigate the plasma properties in the near-Earth environment with high precision, any perturbation to the instruments generated by surface charging represents a concern for science return. Moreover, the charging phenomenon can lead to the development of variable electric and magnetic fields and, in most extreme scenarios, the onset of electrostatic discharges that may cause temporary malfunctions or, in worst cases, mission loss. These discharges occur when the potential difference between near surfaces, exceeds a critical threshold. Such conditions are more likely to occur when the spacecraft structure includes both conductive and dielectric materials. For PMO this risk is expected to remain low, as per baseline the seven spacecrafts will be predominantly conductive, allowing fast charge redistribution. However, as the PMO spacecraft will traverse multiple plasma regions of the Earth’s magnetospheric system during the Key Science Phases (KSPs), evaluating the resulting charging effects is essential. These analyses are crucial not only for PMO but for all space missions, as they support the development of reliable spacecraft designs and ensure safe operation in diverse plasma conditions.

How to cite: Michelagnoli, M., Marcucci, M. F., Retinò, A., Berthomier, M., Khotyaintsev, Y., Eriksson, A., Soucek, J., Johansson, F., Cipriani, F., Focardi, M., and Merola, P.: Preliminary analyses of Surface Charging effects for the Plasma Observatory (PMO) mission, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19522, https://doi.org/10.5194/egusphere-egu26-19522, 2026.

EGU26-20099 | ECS | Orals | ST2.2

In search of multi-scale plasma instabilities at the heart of substorm onset: implications for the Plasma Observatory mission 

Ishbel Carlyle, Jonathan Rae, Andy Smith, Matthew Townson, Clare Watt, Robert Michell, and Marilia Samara

The physical trigger of substorm onset remains one of the key unresolved problems in magnetospheric physics. Understanding how, when, and why stored energy in Earth’s magnetotail is explosively released is central to space-weather science. To identify the instability responsible for detonation, recent studies have focused on the earliest auroral signatures of onset—small-scale, quasi-periodic structures known as auroral beads. Previous work has linked these beads to plasma instabilities and to magnetotail dynamics through kinetic Alfvén waves.

To further understand the substorm onset mechanism, we use new measurements from a narrow-field, high-cadence auroral imager. By extending the Kalmoni et al. (2018) methodology, we track the temporal evolution and dispersion characteristics of “mini beads”, in effect beads-within-beads. Our analysis shows that all types of beads move in the same eastward direction but that mini beads precede the larger beads by at least one minute. However, in contrast to larger-scale beads, mini beads obey different dispersion relations, suggesting that mini beads arise from a distinct physical process and represent an earlier or new stage of the instability development leading to substorm onset.  This means that we need to understand the near-Earth transition region on multiple scales far earlier than currently thought, challenging all current substorm onset paradigms. 

We discuss the implications of this analysis for determining the role of multi-scale physical processes in substorm onset for multi-spacecraft missions such as Plasma Observatory.

How to cite: Carlyle, I., Rae, J., Smith, A., Townson, M., Watt, C., Michell, R., and Samara, M.: In search of multi-scale plasma instabilities at the heart of substorm onset: implications for the Plasma Observatory mission, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20099, https://doi.org/10.5194/egusphere-egu26-20099, 2026.

EGU26-20284 | Orals | ST2.2

Energy exchanges between particles and ion-scale waves and structures in space plasmas with multi-scale explorations: insights from numerical simulations 

Lorenzo Matteini, Petr Hellinger, Luca Franci, Andrea Verdini, Simone Landi, Emanuele Papini, Victor Montagud Camps, Leos Pohl, and Devesh Dhole

 

The crossover between fluid and ion scales in space plasmas plays a crucial role in the overall energization of the system and it’s where most of the energy exchanges between fields and particles take place. At these scales, turbulent dynamics cascading from larger fluid scales and structures from local ion microphysics typically coexist, leading to still unexplored couplings. Multi-point/multi-scale measurements  are then required to fully capture this complex dynamics in situ. 7-point measurements by Plasma Observatory (PMO) in the Earth’s magnetosphere environment offer the opportunity to explore this dynamics and the fluid-ion scale coupling for the first time, in plasma environments with different typical characteristic parameters  and dynamical regimes: e.g. solar wind, magnetosheath, magnetotail.

In this presentation, we review numerical simulations of plasma turbulence focussing on the transition from fluid to ion scales and its coexistence with ion kinetic processes, in particular micro-instabilities (e.g. mirror, firehose, ion-drift). This include the role played by pressure-strain interactions in controlling the turbulent cascade rate and modulating energy exchanges in the plasma, and how these aspects could be captured for the first time by a constellation like PMO.

We address the interplay between these processes and highlight the different spatial and temporal scales involved. As waves and structures from these processes are typically anisotropic, different characteristic scales can be observed, depending on the direction of the sampling, thus making multi-point measurements essential to fully capture them.

How to cite: Matteini, L., Hellinger, P., Franci, L., Verdini, A., Landi, S., Papini, E., Montagud Camps, V., Pohl, L., and Dhole, D.: Energy exchanges between particles and ion-scale waves and structures in space plasmas with multi-scale explorations: insights from numerical simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20284, https://doi.org/10.5194/egusphere-egu26-20284, 2026.

EGU26-20405 | Posters on site | ST2.2

The ion and Electron Plasma Camera of the Plasma Observatory Mission 

Matthieu Berthomier, Gwendal Hénaff, Colin Forsyth, Benoit Lavraud, Vincent Génot, Frédéric Leblanc, Chris Brockley-Blatt, Jean-Denis Techer, Yvon Alata, Evan Seneret, Gabriel Poggia, Alessandro Retino, and Olivier Le Contel

The ion and Electron Plasma Camera (iEPC) onboard the Plasma Observatory mission will provide the 3D velocity distribution function of thermal and supra-thermal ions and electrons in the 10 eV to 25 keV energy range with 12% energy resolution, 22.5° angle resolution, and at 250 ms cadence. It will be deployed on all the 7 satellites of the mission, allowing the first characterization of multi-scale particle acceleration processes in space plasmas. We present the capability of the iEPC instrument concept, which is based on the donut analyser topology (Morel et al., 2017), further optimized for the Plasma Obervatory mission (Hénaff and Berthomier, jgr 2025), and tested at LPP (Hénaff et al, jgr 2025). The iEPC is the first plasma spectrometer with a 3D instantaneous field-of-view with 128 look directions in an energy range relevant for magnetospheric plasmas. Altough being a very compact sensor, the iEPC geometric factor reaches 10-3 cm2.sr.eV/eV per look direction, which will provide excellent counting statistics, even in the dilute magnetospheric plasmas.

How to cite: Berthomier, M., Hénaff, G., Forsyth, C., Lavraud, B., Génot, V., Leblanc, F., Brockley-Blatt, C., Techer, J.-D., Alata, Y., Seneret, E., Poggia, G., Retino, A., and Le Contel, O.: The ion and Electron Plasma Camera of the Plasma Observatory Mission, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20405, https://doi.org/10.5194/egusphere-egu26-20405, 2026.

EGU26-20458 | Posters on site | ST2.2

Multipoint Measurements for Analysis of Physical Fields 

Marcin Grzesiak, Dorota Przepiórka-Skup, Barbara Matyjasiak, and Hanna Rothkaehl

Multipoint measurements offer a powerful framework for dissecting spatiotemporal dynamics in physical fields, particularly in plasma environments. This presentation, tailored to the Cluster-Plasma Observatory Workshop, emphasises applications in ionospheric and magnetospheric studies, with a focus on Cluster mission data.

Notable uses include characterising field structure size and orientation. Ionospheric irregularities have been mapped via GNSS total electron content and LOFAR radio observations . In the magnetosphere, Cluster measurements near the bow shock have revealed nonlinear magnetic structures, demonstrating transferability to vector field deformations.

Drift velocities are derived using correlation and spectral spaced-antenna methods . Drift dispersion follows from scintillation analysis, while Cluster configurations enable wave arrival direction estimation. These techniques also quantify inter-scale energy flows, advancing plasma turbulence models.

Multipoint analysis thus underpins Cluster's legacy in plasma physics, informing space weather and field modeling.

How to cite: Grzesiak, M., Przepiórka-Skup, D., Matyjasiak, B., and Rothkaehl, H.: Multipoint Measurements for Analysis of Physical Fields, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20458, https://doi.org/10.5194/egusphere-egu26-20458, 2026.

EGU26-20725 | ECS | Orals | ST2.2 | Highlight

Numerical Simulations Supporting Plasma Observatory Proposal: Working Group 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 (PMO) proposes a seven-spacecraft constellation, to simultaneously measure plasma characteristics and gradients at both fluid and ion scales simultaneously, to investigate multi-scale cross-coupling processes in the Earth’s magnetosphere and around it. The proposal work is supported by several working groups, one of which is the Group on Simulation Numerical Support (GIANNI). The group 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 PMO constellation parameters. This presentation introduces the group’s models and capabilities, including the wider collaborations with other working groups stemming from the tasks, such as evaluation of multipoint methods from simulation data. Plasma Observatory science objectives are reviewed with a focus towards numerical modelling avenues.

How to cite: Alho, M., Trotta, D., and Valentini, F. and the Plasma Observatory’s Group on Simulation Numerical Support (GIANNI): Numerical Simulations Supporting Plasma Observatory Proposal: Working Group GIANNI, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20725, https://doi.org/10.5194/egusphere-egu26-20725, 2026.

EGU26-20732 | Posters on site | ST2.2

The DPU BOX-P flight software of Plasma Observatory, a LIRA contribution 

Léa Griton, Philippe Plasson, Karine Issautier, Milan Maksimovic, Thibault Peccoux, Pierre-Vincent Gouel, Matthieu Berthomier, Cécile Fiachetti, Hanna Rothkaehl, Grzegorz Ptasinski, Raffaella D'Amicis, Maria Marcucci, and Alessandro Retino

Plasma Observatory is one of the three candidates currently being evaluated by ESA as the future M7 mission. Its objectives are to determine how particles are energized, identify the main processes that transport energy in space plasma, and understand the interactions between the different regions of the Earth's magnetosphere with multi-scale measurements in situ. To achieve these scientific objectives, Plasma Observatory (PMO) is deseigned as seven identical sister spacecrafts (SSCs) in a two nested tetrahedra configuration.

The Laboratory for Instrumentation and Research in Astrophysics (LIRA) of the Observatory of Paris is responsible for the DPU-P application software for the BOX-P instrument. The LIRA contribution includes the specification, design, implementation and testing, verification and validation, product assurance, and development of the test platform. The DPU BOX-P flight software transforms the raw data produced by the instruments into scientific products of L0 level that can be used on the ground (precise dating, synchronisation, filtering, reduction, compression), which means that a significant part of the scientific value of each instrument is directly produced by the software. Responsibility for the flight software places LIRA at the heart of defining scientific products (content, format and cadence of L0s), optimizing on-board processing and science/resource trade-offs, in direct interaction with the instrument teams and mission constraints. The LIRA team has recognized expertise in complex scientific flight software, demonstrated on missions such as PLATO and Solar Orbiter.

Here we present the DPU-P software and we discuss its contribution to the science of Plasma Observatory.

How to cite: Griton, L., Plasson, P., Issautier, K., Maksimovic, M., Peccoux, T., Gouel, P.-V., Berthomier, M., Fiachetti, C., Rothkaehl, H., Ptasinski, G., D'Amicis, R., Marcucci, M., and Retino, A.: The DPU BOX-P flight software of Plasma Observatory, a LIRA contribution, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20732, https://doi.org/10.5194/egusphere-egu26-20732, 2026.

EGU26-22057 | Posters on site | ST2.2

Impact of Turbulence on the Stability and Transport Processes of the Plasma Sheet 

Marina Stepanova, Victor Pinto, Cristóbal Espinoza, Joaquin Diaz Peña, and Elizaveta Antonova

Interaction between a turbulent plasma flow like solar o stellar wind and a magnetic field as an obstacle is very common for space and astrophysical plasmas. The magnetosphere of the Earth is formed precisely as a result of such interaction, and there is a vast amount of evidence suggesting that the geomagnetic tail is like a turbulent wake behind an obstacle. These solar wind turbulent fluctuations are strongly amplified after crossing the bow shock,
forming the plasma flows in the magnetosheath. At the same time, the geomagnetic tail contains the plasma sheet filled by dense and turbulent plasmas and tail lobes filled by a rare quasi-laminar plasmas. The Large-scale vortices in the wake are able to generate turbulent transport that takes place both along the plasma sheet, in the X and Y directions, and across the plasma sheet, in the Z direction. Thus, turbulent fluctuations in all directions should be taken into consideration when analyzing plasma transport in the plasma sheet, and stability of the plasma sheet itself. The interaction between the turbulent plasma sheet and the inner magnetosphere regions is important for understanding of the key magnetospheric processes such as geomagnetic storms and substorms. At the same time, the variations in the solar wind density, velocity, and interplanetary magnetic field consonantly change the plasma conditions both in the plasma sheet and the inner magnetosphere, but due to different and not fully understood mechanisms. Data from CLUSTER, and Themis satellites are used to analyse the stability of turbulent plasma sheet and turbulent transport for different solar wind conditions and geomagnetic activity.The results obtained show that the level of turbulence in the plasma sheet, characterized by the eddy diffusion, correlates with the dawn-dusk electric field, and depends of the solar wind and IMF parameters for both quiet and disturbed geomagnetic conditions.

How to cite: Stepanova, M., Pinto, V., Espinoza, C., Diaz Peña, J., and Antonova, E.: Impact of Turbulence on the Stability and Transport Processes of the Plasma Sheet, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22057, https://doi.org/10.5194/egusphere-egu26-22057, 2026.

EGU26-22228 | Orals | ST2.2

Oblique Drift Instability in Low Beta Plasma 

Mihailo Martinović, Kristopher Klein, Leon Ofman, Yogesh Yogesh, Jaye Verniero, Peter Yoon, Gregory Howes, Daniel Verscharen, and Benjamin Alterman

Parameters of solar wind velocity distributions are well constrained by thresholds of ion-driven plasma instabilities derived from linear theory. Surpassing these thresholds results in the transfer of energy from particles to coherent electromagnetic waves as the system is altered toward a more stable configuration. We use linear Vlasov-Maxwell theory to describe an Oblique Drift Instability (ODI) that constrains the limits of stable parametric space for a low-beta plasma that contains a drifting proton beam or helium population. This instability decreases the relative drift of secondary populations and prevents beta from decreasing below a minimum value by heating both the core and drifting populations. Our predictions are of interest for Parker Solar Probe (PSP) observations, as they provide an additional mechanism for perpendicular heating of ions active in the vicinity of Alfven surface. The ODI may explain the discrepancy between long-standing expectations of measurements of very low-beta plasmas in the near-Sun environment and in situ observations, where beta is consistently measured above 1%. In parallel, it proposes an interpretation why the drift of the secondary ion populations with respect to the bulk of thermal protons is reduced to no more than approximately the local Alfven speed, as observed in earlier PSP encounters.

How to cite: Martinović, M., Klein, K., Ofman, L., Yogesh, Y., Verniero, J., Yoon, P., Howes, G., Verscharen, D., and Alterman, B.: Oblique Drift Instability in Low Beta Plasma, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22228, https://doi.org/10.5194/egusphere-egu26-22228, 2026.

NP4 – Time Series and Big Data Methods

EGU26-1927 | ECS | Orals | NP4.2

Differentiable Atmospheric Modelling with SpeedyWeather.jl  

Maximilian Gelbrecht, Milan Klöwer, Brian Groenke, and Niklas Boers

The current generation of hybrid machine learning and physics-informed machine learning is often limited by the missing availability of comprehensive differentiable models: either strongly simplified models have to be used or machine learning (ML) can’t be integrated natively into process-based models and must be trained separately. Here, we present the ongoing development of SpeedyWeather.jl: A general circulation model that’s differentiable, GPU-capable and ready for ML simulations. SpeedyWeather.jl is a spectral atmospheric GCM with a primitive equation core on flexible grid implementations from Gaussian to HEALPix. It contains simple yet interactive representations of ocean, land and sea ice for coupled climate simulations. With a user interface made for modularity and interactivity, it’s ideally suited as a framework for hybrid atmospheric models. For example, new parameterizations can be defined without any lines of code for GPU or differentiability specifics, yet integrate seamlessly into those. We document the process to achieve differentiability of our model using the general purpose automatic differentiation library Enzyme, problems we encountered and solutions we found. We demonstrate the differentiability with a sensitivity analysis of our model, initial developments of data-driven parameterizations, and give an outlook on the development of differentiable Earth system models. 

How to cite: Gelbrecht, M., Klöwer, M., Groenke, B., and Boers, N.: Differentiable Atmospheric Modelling with SpeedyWeather.jl , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1927, https://doi.org/10.5194/egusphere-egu26-1927, 2026.

EGU26-2240 | Posters on site | NP4.2

Estimating Canopy Resistance Using Machine Learning and Analytical Approaches 

Cheng-I Hsieh, I-Hang Huang, and Chun-Te Lu

Canopy resistance is a key parameter in the Penman–Monteith (P–M) equation for calculating evapotranspiration (ET). In this study, we compared a machine learning algorithm–support vector machine (SVM) and an analytical solution (Todorovic, 1999) for estimating canopy resistances. Then, these estimated canopy resistances were applied to the P–M equation for estimating ET; as a benchmark, a constant (fixed) canopy resistance was also adopted for ET estimations. ET data were measured using the eddy-covariance method above three sites: a grassland (south Ireland), Cypress forest (north Taiwan), and Cryptomeria forest (central Taiwan) were used to test the accuracy of the above two methods. The observed canopy resistance was derived from rearranging the P–M equation. From the measurements, the average canopy resistances for the grassland, Cypress forest, and Cryptomeria forest were 163, 346, and 321 (s/m), respectively. Our results show that both methods tend to reproduce canopy resistances within a certain range of intervals. In general, the SVM model performs better, and the analytical solution systematically underestimates the canopy resistances and leads to an overestimation of evapotranspiration. It is found that the analytical solution is only suitable for low canopy resistance (less than 100 s/m) conditions.

How to cite: Hsieh, C.-I., Huang, I.-H., and Lu, C.-T.: Estimating Canopy Resistance Using Machine Learning and Analytical Approaches, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2240, https://doi.org/10.5194/egusphere-egu26-2240, 2026.

EGU26-2804 | ECS | Orals | NP4.2

AI-generated ensemble river flow forecasting: Using rollout and an additional noise input to build ensemble forecasts 

Karan Ruparell, Kieran Hunt, Hannah Cloke, Christel Prudhomme, Florian Pappenberger, and Matthew Chantry

Machine learning models have been used with success to produce accurate river discharge forecasts at multiple lead times. However, almost no research has been done to show if they are physically consistent across lead times. In the deterministic problem setting, where models output a single forecast with multiple leadtimes, these models are known to be mean-seeking, predicting the most likely river flow for each day, regardless of how likely the resulting trajectory is to occur. This is important for forecasters who need to look at the multi-day properties of a forecast, such as the accumulated flow or number of days over threshold. When each leadtime is described as an independent distribution, the model provides no insight into how to connect the uncertainties at each lead time, as an ensemble forecast would. In this paper, we show that temporal consistency in machine learning forecasts cannot be assumed, and develop two methods for enforcing temporal consistency, the Conditional-LSTM and Seeded-LSTM. Through this, we create ensemble forecasts that successfully predict temporal properties of the 10-day hydrographs. We find that by explicitly training the model to treat the prediction of previous lead times as truth, our model better predicts temporal properties of 10-day hydrographs than other standard methods. Our approach allows users to efficiently generate as many ensemble members as desired, and we use our results to highlight the important of developing temporally consistent ensembles.

How to cite: Ruparell, K., Hunt, K., Cloke, H., Prudhomme, C., Pappenberger, F., and Chantry, M.: AI-generated ensemble river flow forecasting: Using rollout and an additional noise input to build ensemble forecasts, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2804, https://doi.org/10.5194/egusphere-egu26-2804, 2026.

EGU26-3361 | Posters on site | NP4.2

Midlatitude Cyclone Intensity Biases in Machine Learning Weather Prediction Models 

Helen Dacre, Andrew Charlton-Perez, Simon Driscoll, Suzanne Gray, Ben Harvey, Natalie Harvey, Kevin Hodges, Kieran Hunt, and Ambrogio Volonte

Forecasting the location and intensity of strong winds associated with midlatitude cyclones remains a key challenge due to their substantial societal and environmental impacts. In this study, we conditionally evaluate the ability of numerical weather prediction (NWP) models and machine learning weather prediction (MLWP) models to represent wind structures linked to these cyclones. Using a feature‑based tracking approach applied to a large sample of Northern Hemisphere cyclone events, we compare how different modelling frameworks capture cyclone evolution, including track, intensity, and near‑surface wind characteristics.

Our analysis shows that MLWP models can reproduce broad aspects of cyclone behaviour, such as large‑scale track evolution, with skill comparable to established operational NWP forecasting systems at medium-range lead times. However, we also identify systematic differences in how these models represent cyclone intensity and associated wind extremes. In particular, MLWP models tend to underestimate key high‑impact features, such as minimum pressure and peak near‑surface winds, relative to dynamical NWP forecasts.

These findings highlight both the promise and current limitations of MLWP systems for predicting midlatitude cyclone hazards. Understanding these behaviours provides guidance for future model development and for the use of ML‑based forecasts in operational and risk‑focused applications.

 

How to cite: Dacre, H., Charlton-Perez, A., Driscoll, S., Gray, S., Harvey, B., Harvey, N., Hodges, K., Hunt, K., and Volonte, A.: Midlatitude Cyclone Intensity Biases in Machine Learning Weather Prediction Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3361, https://doi.org/10.5194/egusphere-egu26-3361, 2026.

EGU26-4279 | Orals | NP4.2

Online learning of subgrid-scale models for quasi-geostrophic turbulence in planetary interiors 

Alexandre Fournier, Hugo Frezat, and Thomas Gastine

The use of machine learning to represent small-scale processes, such as subgrid-scale (SGS) dynamics, is now well established in weather forecasting and climate modelling. Recent advances have demonstrated that SGS models trained via "online" end-to-end learning - where the dynamical solver operating on the filtered equations participates in the training - can outperform traditional physics-based approaches. However, most studies have focused on idealised periodic domains or spheres, neglecting mechanical boundaries present in systems such as planetary interiors. To address this issue, we introduce a pseudo-spectral differentiable solver for the study of two-dimensional quasi-geostrophic turbulence in a rapidly rotating, axially symmetric bounded domain. A key advantage of the online learning approach is its implicit correction of the commutation errors arising from the irregular Chebyshev grid used in the radial direction, achieved through the estimation of correction terms for the filtered equations. In addition, since Chebyshev polynomials are not boundary-preserving, we project training data extracted from the high-resolution direct numerical simulation (DNS) from the fine grid onto the coarse grid using a Galerkin approach that ensures compatibility with the boundary conditions. 

We examine three configurations, varying the geometry (between an exponential container and a spherical shell) and the rotation rate. The flow is driven by a prescribed analytical forcing that mimics a network of pumps, allowing precise control over the energy injection scale and an exact estimate of the power input. For each case, we evaluate the accuracy of the online-trained SGS model against the reference DNS using integral quantities and spectral diagnostics. In all configurations, we show that an SGS model trained on data spanning only one turnover time remains stable and accurate over integrations at least a hundred times longer than the training period. Moreover, we demonstrate the model's remarkable ability to reproduce slow processes occurring on time scales far exceeding the training duration, such as the inward drift of jets in the spherical shell geometry, which exhibits a quasi-periodic recurrence time of O(10) turnover times. These results suggest a promising path towards developing SGS models for planetary and stellar interior dynamics, including dynamo processes. They indicate that costly DNS may need to be run only for short durations to generate training data, enabling subsequent long-term simulations with the trained model at a negligible computational cost.

 

How to cite: Fournier, A., Frezat, H., and Gastine, T.: Online learning of subgrid-scale models for quasi-geostrophic turbulence in planetary interiors, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4279, https://doi.org/10.5194/egusphere-egu26-4279, 2026.

EGU26-4536 | Orals | NP4.2 | Highlight

Aardvark weather: end-to-end data-driven weather forecasting 

Richard Turner

Weather forecasting is critical for a range of human activities including transportation, agriculture, industry, as well as the safety of the general public. Over the last two years, machine learning models have shown that they have the potential to transform the complex weather prediction pipeline, but current approaches still rely on numerical weather prediction (NWP) systems, limiting forecast speed and accuracy. In this talk, I will give some of the background on these developments. I will then introduce a machine learning model which can replace the entire operational NWP pipeline. Aardvark Weather, an end-to-end data-driven weather prediction system, ingests raw observations and outputs global gridded forecasts and local station forecasts. Further, it can be optimised end-to-end to maximise performance over quantities of interest. I will show that the system outperforms an operational NWP baseline for multiple variables and lead times for gridded and station forecasts. These forecasts are produced with a remarkably simple neural process model using just 8% of the input data and three orders of magnitude less compute than existing NWP and hybrid AI-NWP methods. We anticipate that Aardvark Weather will be the starting point for a new generation of end-to-end machine learning models for medium-range forecasting.

How to cite: Turner, R.: Aardvark weather: end-to-end data-driven weather forecasting, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4536, https://doi.org/10.5194/egusphere-egu26-4536, 2026.

The inherent limitations of individual geophysical methods and the sparsity of observational data often render inversion results unstable and non-unique. Joint inversion of multiphysics data exploits the complementary sensitivities of different physical fields regarding depth, resolution, and boundary features, thereby significantly mitigating the ambiguity of single-method inversion and enhancing interpretation reliability. Traditional joint inversion approaches primarily fall into two categories: spatial structure-based and physical parameter-based constraints. The former relies on the similarity of property distribution patterns, which struggles to decouple non-homologous anomalies, while the latter is often constrained by the unreliability of empirical relationships under complex geological conditions. Recently, deep learning methods based on the U-Net architecture have achieved joint inversion by establishing constraints based solely on spatial structural similarity (Hu et al., 2025) or physical parameter correlations (Guo et al., 2021). Although promising, these methods often fail to accurately characterize non-homologous anomalies in complex geological environments.

This study proposes a dual-stream 3D U-Net architecture incorporating a hybrid attention-gating mechanism. In terms of methodology, we first construct a training dataset based on rock physics data that encompasses both statistical correlations and structural discrepancies. Regarding the network architecture, independent encoders are employed to extract 3D features from gravity and magnetic data, respectively. A cross-attention module is then utilized to capture deep structural correlations, thereby enhancing cooperative inversion in homologous regions. Subsequently, a gated fusion module is introduced as an adaptive feature selector to effectively disentangle inconsistent features in non-homologous regions. Finally, the prediction models are generated through independent decoders.

During the joint inversion implementation phase, the network takes preliminary independent inversion results as input to predict high-fidelity models that integrate physical and geological priors. We incorporate these predicted models as reference models into the regularization term of the joint inversion objective function, constructing a deep-prior-based constraint. During iterative optimization, this constraint guides the inversion trajectory toward the fine geological structures predicted by deep learning by minimizing the discrepancy between the inverted and reference models, while ensuring the fit to observational data. This mechanism achieves an organic integration of data-driven and physics-driven approaches.

References

  • Hu, Y. Su, X. Wu, Y. Huang and J. Chen, "Successive Deep Perceptual Constraints for Multiphysics Joint Inversion," in IEEE Transactions on Geoscience and Remote Sensing, vol. 63, pp. 1-14, 2025, Art no. 5907114. 
  • Guo, H. M. Yao, M. Li, M. K. P. Ng, L. Jiang and A. Abubakar, "Joint Inversion of Audio-Magnetotelluric and Seismic Travel Time Data With Deep Learning Constraint," in IEEE Transactions on Geoscience and Remote Sensing, vol. 59, no. 9, pp. 7982-7995, Sept. 2021.

How to cite: Xi, B. and wang, Z.: A Hybrid Attention-Gating Deep Learning Framework for 3D Joint Inversion of Gravity and Magnetic Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5241, https://doi.org/10.5194/egusphere-egu26-5241, 2026.

EGU26-5888 | Orals | NP4.2

Quantum machine learning-based parametrization for boundary layer turbulence 

Lena Dogra, Janis Klamt, Veronika Eyring, and Mierk Schwabe

In light of the urgent need to accelerate measures for the adaptation to and mitigation of climate change, accurate Earth system models are more important than ever, for technology assessment and the identification of the most effective climate protection strategies. Global climate models have successfully projected consequences of different future scenarios, but the spread in projections remains large, with subgrid-scale parametrizations being the main origin of these uncertainties. Recently, machine learning-based hybrid models have successfully enhanced parametrizations - their directly data-driven structure can more effectively capture the empirical aspects of the parametrizations. Especially for the more complex parametrizations, such as microphysics or turbulence, which we study here, quantum computing could bring decisive further improvements as a part of hybrid models. Atmospheric turbulence strongly affects weather and climate because it determines the rates of exchange of heat, moisture, and momentum between the earth surface and the atmosphere. However, due to the chaotic nature of turbulence and the wide range of turbulent regimes in the atmospheric boundary layer from deep convection to nearly laminar stable conditions, it is notoriously hard to predict and model.
Here, we develop a prototype of a quantum machine learning-based subgrid-scale parametrization for the vertical temperature flux caused by atmospheric turbulence based on semi-idealized Large-Eddy-Simulations. We run experiments with dry convective boundary layers with the PALM model system. The setups span an 8x8 km2 domain with a resolution of 10 m and horizontal periodic boundary conditions and an imposed surface heat flux, combining runs with different surface heat fluxes and geostrophic winds in our training data set. We train quantum and classical neural networks with different architectures, and find that quantum models based on parametrized circuits with just 2 or 3 qubits achieve accuracies similar to classical models with the same number of trainable parameters, highlighting the possibility to use quantum computing for parametrizations in the near future. In contrast, the Smagorinsky closure deviates strongly from the true flux in this setup. Our quantum and classical cell-based models both generalize well to data from PALM runs with unseen parameters close to the seen range. We further analyze the feature importance in quantum and classical models and find that most of our quantum models show better stability of the Shapley values with respect to varying the random initial conditions of the training runs. Since the number of required qubits to capture the idealized setting is low, it is promising to extend our model to more complex settings with realistic topography and varied weather conditions in the future, e.g. by using ICON boundary conditions in PALM, opening the possibility to exploit quantum advantages anticipated by the more stable interpretability of our prototype models.

How to cite: Dogra, L., Klamt, J., Eyring, V., and Schwabe, M.: Quantum machine learning-based parametrization for boundary layer turbulence, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5888, https://doi.org/10.5194/egusphere-egu26-5888, 2026.

EGU26-6079 | Posters on site | NP4.2

Emulating transient climate simulations with generative AI  

Kirien Whan, Karin van der Wiel, and Nikolaj Mücke

Global climate models (GCMs), like KNMI’s EC-Earth, are an important tool to study the global climate system, and to understand how the climate responds to changes in external forcing. Large ensembles of climate simulations are necessary to separate the forced response from fluctuations due to the climate system’s internal variability (Maher et al., 2021; Muntjewerf et al, 2023). GCMs are computationally very expensive to run, particularly as they move towards the km-scale, which makes generating large ensembles very expensive. 

The generative modelling framework allows the transformation of a base distribution to the target distribution and easily facilitates the construction of large ensembles. We compare two generative models: 1) “stochastic interpolants”, that learn a pseudo-time dependent stochastic process that directly interpolates between the current state and the conditional target state of interest, and 2) a “flow matching” model, that learns a pseudo-time dependent deterministic process, conditioned on the current state, between a Gaussian distribution and the target state of interest.  Both models use a PDE-transformer backbone (Holzschuh et al, 2025). 

We train an emulator to predict global 2m-temperature at time t+1 using the previous 5 days of temperature, the annual global mean temperature and some static spatial and temporal features as conditioning inputs. We make predictions auto-regressively, feeding each prediction back into the model to generate sequences of arbitrary length at inference time. We use Large Ensembles from the EC-Earth3 model, for which a transient 16-member (1950-2166) ensemble and two 160-member time slices (2000-2009, 2075-2085) are available (Muntjewerf et al., 2023). The training dataset consists of up to 5 transient members and we use a single member for validation during training. We use another member for inference to produce an ensemble of global temperature simulations.  

The flow matching model successfully generates a stable ensemble of temperature fields that simulates the long-term forced trend, interannual variability, and spatial patterns of (global) temperature similarly to the GCM. 

 

 

References: 

Maher, N., Milinski, S. and Ludwig, R., 2021. Large ensemble climate model simulations: introduction, overview, and future prospects for utilising multiple types of large ensemble. Earth System Dynamics, 12(2), pp.401-418. 

Muntjewerf, L., Bintanja, R., Reerink, T. and Van Der Wiel, K., 2023. The KNMI Large Ensemble Time Slice (KNMI–LENTIS), Geosci. Model Dev. 16 4581–4597. doi: 10.5194. 

Holzschuh, B., Liu, Q., Kohl, G., & Thuerey, N. (2025). PDE-Transformer: Efficient and Versatile Transformers for Physics Simulations. arXiv preprint arXiv:2505.24717. 

How to cite: Whan, K., van der Wiel, K., and Mücke, N.: Emulating transient climate simulations with generative AI , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6079, https://doi.org/10.5194/egusphere-egu26-6079, 2026.

EGU26-6950 | ECS | Orals | NP4.2

Improving AIFS Forecast Skill through Fine-Tuning across Spatial Resolutions and Datasets 

Gabriel Moldovan, Ana Prieto Nemesio, Ewan Pinnington, Simon Lang, Jan Polster, Cathal O'Brien, Mario Santa Cruz, Mihai Alexe, Harrison Cook, Richard Forbes, and Matthew Chantry

Over the past two years, ECMWF has rapidly developed and operationalised two machine-learned forecasting systems: AIFS Single, a deterministic model, and AIFS-ENS, a fully probabilistic forecasting system. Both systems are trained on ERA5 reanalysis data and further fine-tuned using operational IFS analyses. In this talk, we briefly introduce the AIFS framework and present ongoing research aimed at further improving its forecast skill.

Current efforts are driven by several research directions, including increasing spatial resolution and incorporating observational data. The current AIFS models operate at the native ERA5 resolution of approximately 30km. While higher resolutions could significantly improve forecast skill in surface variables, available datasets, such as the operational IFS analysis at 9km, are only available for a limited number of years. To address this, we explore a cross-resolution fine-tuning strategy in which AIFS is first pretrained on ERA5 at coarse resolution and subsequently fine-tuned on six years of recent operational IFS analyses at 9 km. We present promising early results showing that this approach enables stable fine-tuning down to 9 km and leads to significant gains in surface forecast skill.

A second research direction investigates the use of alternative datasets to improve total precipitation forecasts. ERA5 is known to exhibit deficiencies in the representation of precipitation, particularly in the tropics. We therefore fine-tune AIFS using the Integrated Multi-satellitE Retrievals for GPM (IMERG) dataset, which has been shown to better capture precipitation characteristics in this region. Early results indicate that incorporating IMERG data can significantly improve total precipitation forecast skill in AIFS, with the largest benefits observed, as expected, in tropical regions.

How to cite: Moldovan, G., Prieto Nemesio, A., Pinnington, E., Lang, S., Polster, J., O'Brien, C., Santa Cruz, M., Alexe, M., Cook, H., Forbes, R., and Chantry, M.: Improving AIFS Forecast Skill through Fine-Tuning across Spatial Resolutions and Datasets, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6950, https://doi.org/10.5194/egusphere-egu26-6950, 2026.

Machine learning is increasingly used to analyze, predict, and interpret Earth-system behavior. Here we synthesize AI4OCEANS research to identify practical, transferable lessons for developing ML methods that remain robust when applied to real Earth-system data and are evaluated across regions, scales, and event types. We present methodological advances and common pitfalls encountered when building ML workflows for prediction and diagnosis across oceanic and atmospheric contexts. Emphasis is placed on (i) constructing physically meaningful predictors and representations that generalize beyond a single region or period, (ii) designing evaluation strategies that reflect scientific and decision-relevant objectives (including event- and regime-aware metrics where appropriate), and (iii) quantifying uncertainty and interpretability in ways that support scientific insight rather than purely empirical skill. We further discuss when hybrid strategies—combining statistical learning with physical constraints or dynamical context—improve robustness in specific applications. By framing diverse studies through shared methodological questions across geophysical systems (from coastal ocean change through high-impact atmospheric events and into bycatch threats to marine wildlife), the produced frameworks provide guidance for ML development that is directly relevant to Earth-system modelling and prediction, particularly for variability, extremes, and environmental risks and impacts under anthropogenic influences.

How to cite: Nieves, V.: Transferable Machine-Learning Practices for Earth-System Prediction and Diagnosis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7654, https://doi.org/10.5194/egusphere-egu26-7654, 2026.

EGU26-8225 | ECS | Orals | NP4.2

Parameterised PINNs for water infiltration in unsaturated soils 

Mohamed Gowely and Anil Yildiz

Modelling water infiltration in unsaturated soils is vital for maintaining a healthy ecosystem, analysing the stability of slopes, or promoting sustainable agriculture. Recently, Physics-informed Neural Networks (PINNs) have gained popularity in solving highly nonlinear problems like the Richardson-Richards equation (RRE), by approximating physical laws with a loss term in a mesh-free approach, often using sparse data points, to mimic the gap spacing between field sensors. However, despite several successful applications in modelling 1D infiltration problems, the generalisation capability of these models is often limited by the specific scenarios used during training. Therefore, potential of the neural networks as universal approximators are not exploited in such applications. This paper investigates the feasibility of applying a Parameterised-PINNs (P-PINNs) as a surrogate model to solve the RRE. The model was trained only once across a range of infiltration conditions defined by varying soil hydraulic properties and meteorological conditions to evaluate its ability to predict various scenarios within the multidimensional parameter space without additional observation data. Results show that a wider rather than a deeper network architecture, enhanced by dynamic adaptive techniques, such as time-stratified Residual-based Adaptive Refinement (RAR), Layer-wise Locally Adaptive Activation Function (L-LAAF), and Principled Loss Function (PLF), aids in capturing the correct physical profile. Although the model achieved high overall performance when validated against analytical solutions, Nash-Sutcliffe Efficiency (NSE) > 0.99, it exhibited very minor phase errors. P-PINN was tested across drastically changing parameters, e.g. soils with very high or very low air-entry values, and satisfactory validation metrics were obtained. Our implementation P-PINNs demonstrate the potential as a universal non-linear approximator for such problems, where the initial computational cost of training is offset by the instant large-scale evaluations.

How to cite: Gowely, M. and Yildiz, A.: Parameterised PINNs for water infiltration in unsaturated soils, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8225, https://doi.org/10.5194/egusphere-egu26-8225, 2026.

EGU26-8476 | ECS | Orals | NP4.2

CTM-Assisted Generative AI Framework for Satellite-to-Surface Estimation of Ground-Level Air Pollutants 

Hyeonseo Kim, Eunhye Kim, Yoon-Hee Kang, Seongeun Jeong, Soontae Kim, Hyun Cheol Kim, and Rackhun Son

 Accurate monitoring of ground-level air pollutants is essential for exposure assessment and air quality management, but conventional modeling approaches exhibit significant limitations. Chemical Transport Models (CTMs) are computationally intensive and prone to systematic bias, while data-driven models often lack physical consistency and poorly represent long-range transport. To address these limitations, we present a novel hybrid modeling framework with three key innovations. First, satellite retrievals are employed as primary predictors rather than CTM outputs, thereby reducing computational demands. Second, a dual-target learning strategy prioritizes satellite-to-surface relationships, while CTM outputs are incorporated as soft physical constraints in data-sparse regions. Third, a generative diffusion model is integrated to improve the representation of long-range pollutant transport. Focusing on nitrogen dioxide (NO2), the completed framework achieves superior daily predictive accuracy (R2 = 0.72, RMSE = 3.70 ppb), outperforming precursor models. Its successful extension to sulfur dioxide (SO2) and fine particulate matter (PM2.5) demonstrates broad applicability. This study provides a physically informed and computationally efficient solution for scalable generation of high-fidelity, spatially continuous ground-level air quality fields.

This work was funded by the Korea Meteorological Administration Research and Development Program under Grant RS-2024-00404042 and the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (RS-2024-00343921).

How to cite: Kim, H., Kim, E., Kang, Y.-H., Jeong, S., Kim, S., Kim, H. C., and Son, R.: CTM-Assisted Generative AI Framework for Satellite-to-Surface Estimation of Ground-Level Air Pollutants, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8476, https://doi.org/10.5194/egusphere-egu26-8476, 2026.

EGU26-9777 | ECS | Orals | NP4.2

Mapping Ecosystems in the Peruvian Andes Using Hyperspectral Imagery and Machine Learning 

Daria-Ioana Radu, Hugo Lepage, Eustace Barnes, and Crispin Barnes

Mapping the Peruvian Andes has high ecological value because its ecosystems are immensely diverse. These mountains shelter numerous endemic species that could be protected if informed decisions are made when delineating conservation zones. Rigorous analysis of high-altitude regions traditionally requires multiple field visits, which place a financial burden on research teams. Such visits can pose safety risks, as several remote areas are difficult to access on foot due to the steep gradients, cloud cover, and logistical limitations.

Recent advances in satellite missions and machine learning (ML) allow land-cover features to be characterised with fewer ground-truthing expeditions, by utilising patterns present in large imagery datasets. However, the Andes remain challenging to map, because of the spectral similarity among some land-use and land-cover (LULC) classes and because steep gradients can lead to geometric distortions in the recorded images. 

This study highlights an easy-to-use method for generating LULC map prototypes for high-altitude Andean regions using EnMAP and EMIT hyperspectral imagery (HSI). Machine learning algorithms (e.g., K-means clustering, principal component analysis) were applied to the HSI to generate clusters and extract features with high discriminant power among LULC types. Expert interpretation allowed pairing the obtained clusters with suitable ecosystem labels, producing prototype LULC maps.

How to cite: Radu, D.-I., Lepage, H., Barnes, E., and Barnes, C.: Mapping Ecosystems in the Peruvian Andes Using Hyperspectral Imagery and Machine Learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9777, https://doi.org/10.5194/egusphere-egu26-9777, 2026.

EGU26-11323 | ECS | Posters on site | NP4.2

Disentangled and interpretable feature extraction of the Earth electron radiation belt: a first step towards the development of a reduced order model 

Gautier Nguyen, Antoine Brunet, Maria Tahtouh, Guillerme Bernoux, Nourallah Dahmen, and Ingmar Sandberg

The radiation belts are populations of energetic particles, such as electrons and protons, trapped in the near-Earth space vicinity by the geomagnetic field. Because they cover the great majority of existing orbits and because the particles’ dynamics, highly coupled with solar activity, can strongly affect spacecraft components and mission, the accurate modeling of these regions is of uttermost importance for the monitoring of the near-Earth space dynamics.

Traditionally, the radiation belts are modeled by solving a three‑dimensional diffusion equation with numerical solvers. While a single 3D simulation can easily be run in real time, as done routinely in many space weather forecasting pipelines, the computational burden can become significant when the model is used in ensemble‑based data assimilation that potentially requires hundreds of runs, over very long periods, such as those needed for space‑climate studies.

Within this context, machine learning based Reduced Order models (ROMs) offer an interesting solution to approach the solutions of traditional high-fidelity physics-based models with a reasonable accuracy and at a reduced computational cost. This is achieved by projecting project highly non-linear features onto a disentangled, interpretable latent space of reduced dimension which dynamics could be driven by external variables.

In this work, we take a first step towards the development of a ROM for the Earth electron radiation belts. Using a Distance regularized Siamese twin autoencoder (DIRESA) on long-term simulations we manage to reduce electron fluxes on a refined grid to a small subset of latent variables. We then show that these variables that can all be linked with external geomagnetic parameters. This allows them to be at the core of a ROM of the Earth electron radiation belts driven by those external parameters.

This work was supported by both the "Event-Based Electron Belt Radiation Storm Environments Modelling" Activity led by the Space Applications & Research Consultancy (SPARC) under ESA Contract 4000141351/23/UK/EG and ONERA internal fundings, through the federated research project PRF-FIRSTS.

How to cite: Nguyen, G., Brunet, A., Tahtouh, M., Bernoux, G., Dahmen, N., and Sandberg, I.: Disentangled and interpretable feature extraction of the Earth electron radiation belt: a first step towards the development of a reduced order model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11323, https://doi.org/10.5194/egusphere-egu26-11323, 2026.

EGU26-11736 | ECS | Orals | NP4.2

Towards a mass-conservative global sea ice emulator that generalizes across climates 

William Gregory, Mitchell Bushuk, James Duncan, Elynn Wu, Adam Subel, Spencer Clark, Jeremy McGibbon, Brian Henn, Troy Arcomano, W. Andre Perkins, Anna Kwa, Oliver Watt-Meyer, Alistair Adcroft, Chris Bretheron, and Laure Zanna

We introduce FloeNet, a data-driven emulator architecture trained on the Geophysical Fluid Dynamics Laboratory (GFDL) global sea ice model, SIS2. FloeNet is an auto-regressive graph neural network (GNN) which marks a step forward in sea ice emulation as the first model to dynamically evolve the state of sea ice and snow-on-sea-ice by mass and area budget decompositions. Specifically, FloeNet receives mechanical and thermodynamic forcing inputs from the atmosphere and ocean, and predicts ice and snow mass tendencies due to growth, melt, and advection. This yields a mass-conservative and interpretable model, as timestep-to-timestep changes in sea ice area and mass can now be attributed to each term in their respective budget.

Sea ice is often seen as a barometer for climate change. It is therefore crucial that data-driven sea ice models show an accurate response to different climate forcings. To this end, we show how FloeNet successfully reproduces sea ice trends and variability of pre-industrial and 1% CO2 climates, despite being trained only on a present-day climate; FloeNet also reaches globally ice-free conditions under 1% CO2 forcing, with consistent timing to that of the original numerical model. In summary, FloeNet is a fast global sea ice emulator, taking 4.75 hours to generate a 140-year simulation on 1 GPU. It is also stable and accurate, reproducing critical features of long-term sea ice evolution under different forcings. We expect that FloeNet will substantially improve the representation of atmosphere-ice-ocean interactions in existing climate emulators.

How to cite: Gregory, W., Bushuk, M., Duncan, J., Wu, E., Subel, A., Clark, S., McGibbon, J., Henn, B., Arcomano, T., Perkins, W. A., Kwa, A., Watt-Meyer, O., Adcroft, A., Bretheron, C., and Zanna, L.: Towards a mass-conservative global sea ice emulator that generalizes across climates, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11736, https://doi.org/10.5194/egusphere-egu26-11736, 2026.

EGU26-11847 | ECS | Posters on site | NP4.2

Measurement-Constrained Reduced-Order Surrogates for Flexible-Mesh Coastal Ocean Models 

Melissa Ulsøe Jessen, Jesper Sandvig Mariegaard, and Freja Høgholm Petersen

Reduced-order surrogate models based on Koopman autoencoders have recently shown strong potential for accelerating flexible-mesh coastal ocean simulations while maintaining physically meaningful dynamics. In this contribution, we extend a previously validated Koopman autoencoder framework by explicitly incorporating information from in-situ measurements during training.

The proposed approach augments the surrogate training objective with measurement-based constraints, penalizing deviations from observed water surface elevations at selected locations and times. This enables the surrogate to remain consistent with sparse observations while preserving the learned large-scale dynamical structure driven by meteorological forcing and boundary conditions.

The method is evaluated on two realistic MIKE 21 HD coastal-ocean configurations published as open WaterBench datasets: the Southern North Sea and the Øresund Strait. Performance is assessed against both full physics-based simulations and independent in-situ observations, focusing on accuracy, temporal stability, and generalization beyond the training period.

Results demonstrate that measurement-constrained training can reduce local prediction errors near observation points without degrading global performance, while retaining the substantial inference speed-ups characteristic of Koopman-based reduced-order models. The proposed framework represents a step toward tighter integration of observations and machine-learning surrogates for efficient, observation-aware coastal ocean modelling, with relevance for ensemble forecasting and long-term scenario analysis.

How to cite: Jessen, M. U., Mariegaard, J. S., and Petersen, F. H.: Measurement-Constrained Reduced-Order Surrogates for Flexible-Mesh Coastal Ocean Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11847, https://doi.org/10.5194/egusphere-egu26-11847, 2026.

EGU26-12000 | ECS | Posters on site | NP4.2

Representing Subgrid-Scale Cloud Effects in a Radiation Parameterization using Machine Learning 

Katharina Hafner, Sara Shamekh, Guillaume Bertoli, Axel Lauer, Robert Pincus, Julien Savre, and Veronika Eyring

Improvements of Machine Learning (ML)-based radiation emulators remain constrained by the underlying assumptions to represent horizontal and vertical subgrid-scale cloud distributions, which continue to introduce substantial uncertainties. In this study, we introduce a method to represent the impact of subgrid-scale clouds by applying ML to learn processes from high-resolution model output with a horizontal grid spacing of 5km. In global storm resolving models, clouds begin to be explicitly resolved. Coarse-graining these high-resolution simulations to the resolution of coarser Earth System Models yields radiative heating rates that implicitly include subgrid-scale cloud effects, without assumptions about their horizontal or vertical distributions. We define the cloud radiative impact as the difference between all-sky and clear-sky radiative fluxes, and train the ML component solely on this cloud-induced contribution to heating rates. The clear-sky tendencies remain being computed with a conventional physics-based radiation scheme. This hybrid design enhances generalization, since the machine-learned part addresses only subgrid-scale cloud effects, while the clear-sky component remains responsive to changes in greenhouse gas or aerosol concentrations. Applied to coarse-grained data offline, the ML-enhanced radiation scheme reduces errors by a factor of up to 4-10 compared with a conventional coarse-scale radiation scheme. We observe improved radiative heating rates across several cloud regimes and regions, including precipitating and non-precipitating clouds and stratocumulus regions. This shows the potential of representing subgrid-scale cloud effects in radiation schemes with ML for the next generation of Earth System Models.

How to cite: Hafner, K., Shamekh, S., Bertoli, G., Lauer, A., Pincus, R., Savre, J., and Eyring, V.: Representing Subgrid-Scale Cloud Effects in a Radiation Parameterization using Machine Learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12000, https://doi.org/10.5194/egusphere-egu26-12000, 2026.

EGU26-12760 | ECS | Posters on site | NP4.2

Evaluating the forecast skill of machine-learning weather prediction models across a selection of extreme UK windstorms 

James Hewitt, Ambrogio Volonté, Ben Harvey, Andressa Andrade Cardoso, Kieran Hunt, Natalie Harvey, Oscar Martinez-Alvarado, Suzanne Gray, Helen Dacre, and Kevin Hodges

While numerical weather prediction (NWP) underpins existing early warning systems, its high computational cost limits scalability. Machine-learning weather prediction (MLWP) offers a promising alternative, yet its skill and reliability at forecasting wind extremes and small-scale storm features across different storms remain uncertain. Evaluating the forecast skill of MLWP models across a range of storms is therefore critical before MLWP can be integrated safely into early warning systems.

 

This study evaluates the performance of eight leading MLWP models at forecasting the peak 10 m and 850 hPa wind speeds, pressure minima, and relative vorticity associated with the most damaging UK windstorms from the 2023/24 winter season: Babet, Ciarán, Debi, Gerrit, Henk and Isha. MLWP models are evaluated against ERA5 and IFS analysis and benchmarked against the NWP IFS ensemble forecast. The results reveal substantial variability in MLWP forecasting skill both between storms and across models.

 

MLWP forecast skill is found to be linked to the horizontal scale and dynamical nature of the storm feature producing the strongest winds. While wind maxima associated with large-scale conveyor-belt airstreams are generally well predicted, those arising from smaller-scale features, including the cold conveyor belt and sting jets, are underestimated. MLWP model performance is also found to be variable between storms, with no clear best- or worst-performing model. The higher-resolution Aurora-0.1 model is not found to be better at forecasting wind extremes, despite the small spatial scale of the storm features producing the strongest winds in four of the storms analysed.

 

An in-depth, feature-based analysis is performed for Storms Henk and Isha. Henk proved challenging for both MLWP and NWP models to forecast, resulting in short-notice and inaccurate wind alerts from the Met Office. The MLWP models performed worst for Isha overall, despite the NWP models predicting it well. Across both storms, MLWP models struggled to predict small-scale features associated with extreme winds and tended to smooth sharp frontal gradients.

 

These results highlight critical limitations in existing MLWP models that make them unsuitable for replacing NWP as a primary forecasting tool for hazardous UK windstorms today. However, current MLWP models could provide rapid, low-cost ensemble information that complements traditional NWP outputs, or serve as a part of a hybrid ML-NWP approach, particularly if structural limitations in representing fine-scale wind maxima are acknowledged and mitigated.

How to cite: Hewitt, J., Volonté, A., Harvey, B., Andrade Cardoso, A., Hunt, K., Harvey, N., Martinez-Alvarado, O., Gray, S., Dacre, H., and Hodges, K.: Evaluating the forecast skill of machine-learning weather prediction models across a selection of extreme UK windstorms, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12760, https://doi.org/10.5194/egusphere-egu26-12760, 2026.

EGU26-13711 | ECS | Orals | NP4.2

Physics-informed, open-box neural network parameterization of moist physics 

Peter Ukkonen and Hannah Christensen

Machine learning hold the promise of unlocking more accurate and realistic parameterizations of atmospheric processes, but brings its own set of challenges and drawbacks. Among top issues are generalization, stability and interpretability. Here we present a parameter-efficient neural network parameterization which aims to address these issues by incorporating physical knowledge to a high degree. By predicting fluxes and microphysical process rates instead of total tendencies, the conservation of water can be hardcoded, which is shown to improve online performance. Furthermore, a physically motivated architecture based on vertically recurrent neural networks enables high computational efficiency and a low number of parameters. The models are trained and evaluated using a superparameterization setup with real orography. The impact of incorporating stochasticity is also discussed. 

How to cite: Ukkonen, P. and Christensen, H.: Physics-informed, open-box neural network parameterization of moist physics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13711, https://doi.org/10.5194/egusphere-egu26-13711, 2026.

EGU26-14578 | ECS | Orals | NP4.2

Machine Learning and Remote Sensing Projections for Peruvian Glaciers (2016–2100) 

Hugo Lepage, Darina Andriychenko Leonenko, Nina Elliott, and Crispin Barnes

The Peruvian Andes contain over 70% of the world's tropical glaciers, which are vital for regional water security and are rapidly destabilising due to climate change. Current large-scale projections often lack the spatial resolution required for localised glacial melt modelling or rely on climate reanalysis products that are too coarse in rugged terrain. This study introduces a unified framework that combines high-resolution remote sensing (Sentinel-2, Landsat-8) with machine learning to characterise, monitor, and forecast glacial evolution across Peru from 2016 to 2100.

We propose a machine-learning modelling approach that addresses both the where and when of glacial retreat. We developed a spatial Random Forest classifier to generate country-wide melt vulnerability maps. Ensemble analysis of driving parameters reveals that "distance-to-edge" and topographic factors (elevation, slope) are significantly stronger predictors of melt spatiality than available coarse-resolution temperature and precipitation datasets. Our spatial model achieves a 74.9% overlap accuracy between simulated and observed melt (2016–2023), nearly doubling the performance of benchmark Multi-Criteria Decision Analysis methods (39.3%).

Complementing this spatial analysis, we developed a temporal, area-based melt model from annual inventories of over 2,000 individual glacier polygons. Using a Huber regression to fit negative power laws to ablation rates, we identified a clear acceleration in retreat for smaller ice bodies, consistent with albedo-ice feedback mechanisms. Between 2016 and 2023, we observed a relative area loss of 15 ± 4% (180 ± 70 km2).

Integrating these models to forecast future scenarios, we project that only ~30% (26–43%) of the 2020 glacial surface area will remain by 2100, with several cordilleras facing near-total extinction. This workflow establishes a new standard for observation-based, scalable glacial modelling, providing the high-resolution spatial and temporal insights necessary for effective water resource management and adaptation strategies in the tropical Andes.

How to cite: Lepage, H., Andriychenko Leonenko, D., Elliott, N., and Barnes, C.: Machine Learning and Remote Sensing Projections for Peruvian Glaciers (2016–2100), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14578, https://doi.org/10.5194/egusphere-egu26-14578, 2026.

EGU26-14900 | ECS | Orals | NP4.2

A Hybrid FNO-Diffusion Framework for Uncertainty-Aware Source Energy Estimation in Atmospheric Waveguides 

Elodie Noëlé, Filippo Gatti, Didier Clouteau, Christophe Millet, and Fanny Lehmann

Estimating the source of acoustic waves propagating in a vertically stratified medium poses significant challenges due to the high variability of the acoustic fields at long-range distances caused by heterogeneous vertical sound speed profiles. This renders the problem an inverse and ill-posed one. To address this challenge, we propose a three-step approach utilizing a Bayesian framework. First, we show that using only the low-frequency components (up to 1.5 Hz) of the acoustic fields is sufficient to capture the source parameters. Second, we develop a fast surrogate forward model based on a Fourier Neural Operator (FNO) [1] to bypass the computational burden of traditional numerical solvers. Finally, we trained diffusion models to represent the complex prior [2] of the atmospheric profiles and to accurately estimate the posterior distribution [3] in the context of our inference problem. The models are trained on a database comprising over 20,000 simulations generated using a normal mode code [4]. Our results show that our FNO model achieves a relative least squares error of approximately 8%. The combined FNO and diffusion model framework [5] is demonstrated to yield more reliable energy estimates when compared to the utilization of the FNO framework alone.

[1] N. Perrone, F. Lehmann, H. Gabrielidis, S. Fresca, and F. Gatti, “Integrating Fourier Neural Operators with Diffusion Models to improve Spectral Representation of Synthetic Earthquake Ground Motion Response,” arXiv preprint arXiv:2504.00757, 2025. doi: 10.48550/arXiv.2504.00757

[2] F. Lehmann, F. Gatti, M. Bertin, and D. Clouteau, “3D elastic wave propagation with a Factorized Fourier Neural Operator (F-FNO),” Computer Methods in Applied Mechanics and Engineering, vol. 417, art. no. 116718, 2023. doi: 10.1016/j.cma.2023.116718

[3] F. Bergamin, C. Diaconu, A. Shysheya, P. Perdikaris, J. M. Hernández-Lobato, R. E. Turner, and E. Mathieu, “Guided Autoregressive Diffusion Models with Applications to PDE Simulation,” in ICLR 2024 Workshop on AI4DifferentialEquations In Science, 2024. 

[4] T. Karras, M. Aittala, S. Laine, and T. Aila, “Elucidating the design space of diffusion-based generative models,” in Proceedings of the 36th International Conference on Neural Information Processing Systems (NeurIPS), 2022, pp. 26565–26577. doi: 10.5555/3600270.3602196

[5] M. Bertin, C. Millet, and D. Bouche, “A low-order reduced model for the long range propagation of infrasound in the atmosphere,” The Journal of the Acoustical Society of America, vol. 136, no. 5, pp. 2693–2705, 2014. doi: 10.1121/1.4896776

How to cite: Noëlé, E., Gatti, F., Clouteau, D., Millet, C., and Lehmann, F.: A Hybrid FNO-Diffusion Framework for Uncertainty-Aware Source Energy Estimation in Atmospheric Waveguides, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14900, https://doi.org/10.5194/egusphere-egu26-14900, 2026.

High-resolution and temporally consistent satellite observations are essential for effectively monitoring, modeling, and mitigating environmental challenges. However, optically based remote sensing faces cross-sensor interoperability issues and is inherently affected by cloud contamination and atmospheric interference, resulting in temporal discontinuities that limit the availability of timely and uninterrupted observations. Existing approaches have primarily focused on retrospective gap-filling of missing data. In contrast, forecasting surface dynamics introduces additional challenges, particularly the need for high-fidelity and temporally continuous information to support near-real-time monitoring and predictive applications as the time since the last observation increases.

To address this challenge, we developed a physics-guided transformer framework trained on Harmonized Landsat, Sentinel-2, and PlanetScope (HLSP) data to forecast uninterrupted daily 30-m surface reflectance during periods with missing optical observations. HLSP is a radiometrically and geometrically harmonized multi-sensor optical dataset integrating Landsat 8–9, Sentinel-2, and PlanetScope imagery to provide sensor-agnostic, temporally consistent surface reflectance products. The model was trained using a multi-year (2017–2025) archive of HLSP surface reflectance imagery across eight agricultural regions in the United States, Brazil, France, Spain, Egypt, South Africa, Thailand, and China. Spectral features from daily HLSP data (30 m resolution) were combined with daily land surface temperature (LST) and soil water content (SWC) at 100-m resolution derived from passive microwave observations. Additional temporal covariates, including day-of-year encoded using sine and cosine transformations, were incorporated to explicitly represent seasonal and phenological timing and enable the network to capture key biophysical, hydroclimatic, and seasonal controls on surface reflectance dynamics.

The physics-guided framework constrains predictions using land–surface energy balance relationships linking surface reflectance, land surface temperature, and soil moisture. These constraints promote physically consistent interactions among surface variables while learning temporally coherent surface reflectance dynamics associated with vegetation growth, moisture persistence, and land–surface energy exchanges.

Model skill was evaluated using RMSE and MAE under a forward-looking temporal validation strategy, in which the model was trained on eight years of historical HLSP data and used to forecast surface reflectance over multiple lead times (2, 5, 10, 15, and 20 days) following the last available optical observation in the final year. Forecasts were validated against independently observed HLSP data for the corresponding periods, allowing assessment of skill degradation as forecast horizons increased. Results demonstrate that incorporating LST, SWC, NDVI, and time-related covariates substantially improves forecast stability and fidelity, particularly under variable climatic and land-cover conditions. The proposed approach provides a scalable and generalizable machine-learning framework for short-term forecasting of EO surface reflectance time series, with applications in climate-impact assessment, drought monitoring, evapotranspiration modeling, and carbon–water flux analysis.

How to cite: Alamdar, S. and Houborg, R.: Physics-Guided Transformer-based Forecasting of High-Resolution Earth Observation Surface Reflectance Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14919, https://doi.org/10.5194/egusphere-egu26-14919, 2026.

EGU26-14956 | ECS | Orals | NP4.2

Super-Resolving Any Place on Earth - Implicit Neural Representations for Sentinel-2 Time Series 

Sander Jyhne, Christian Igel, Morten Goodwin, Per-Arne Andersen, Serge Belongie, and Nico Lang

High-resolution imagery is limited by sensor technology, atmospheric effects, and acquisition costs. This is a well-known challenge in satellite remote sensing, but it also applies to ground-level imaging with handheld devices such as smartphones. Super-resolution seeks to overcome these limitations by enhancing image resolution algorithmically. Single-image super-resolution, however, is an ill-posed inverse problem and therefore depends on strong priors, typically learned from high-resolution training data or imposed through auxiliary information such as high-resolution guidance from another modality. While these methods often produce visually appealing results, they are prone to hallucinating structures that do not reflect the true scene content.

Multi-image super-resolution (MISR) addresses this issue by exploiting multiple low-resolution views of the same scene that are captured with sub-pixel shifts. In this work, we introduce SuperF, a test-time optimization approach for MISR based on coordinate-based neural networks, also known as neural fields. By representing images as continuous signals using implicit neural representations (INRs), neural fields are well suited for reconstructing high-resolution images from multiple aligned observations. The central idea of SuperF is to share a single INR across all low-resolution frames while jointly optimizing the image representation and the sub-pixel alignment between frames.

Compared to prior INR-based approaches adapted from burst fusion and layer separation, SuperF directly parameterizes the sub-pixel alignment using optimizable affine transformation parameters and performs the optimization on a super-sampled coordinate grid corresponding to the target output resolution. We evaluate the proposed method on simulated bursts of satellite imagery as well as on ground-level images captured with handheld cameras, and observe consistent improvements for upsampling factors of up to 8. A key advantage of SuperF is that it operates entirely at test time and does not rely on any high-resolution training data.

How to cite: Jyhne, S., Igel, C., Goodwin, M., Andersen, P.-A., Belongie, S., and Lang, N.: Super-Resolving Any Place on Earth - Implicit Neural Representations for Sentinel-2 Time Series, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14956, https://doi.org/10.5194/egusphere-egu26-14956, 2026.

The primary challenge in forecasting the Earth's magnetic field lies in capturing rapid, non-linear events like geomagnetic jerks. Conventional models relying solely on geomagnetic data often struggle to replicate the variation of those abrupt changes, such as the 2014–2015 geomagnetic jerk.

This study introduces a multiple data approach that simultaneously co-estimates geomagnetic snapshots and Length-of-Day (LOD) variations using a machine learning method. Specifically, we use an Extended Kalman Filter-trained Recurrent Neural Network (EKF-RNN; Sato et al., in press) to model the complex, non-linear dynamics of the Earth's core, including the geomagnetic jerks.

The training and validation datasets for our neural network were derived from the MCM geomagnetic field model (Ropp & Lesur, 2023), which is based on vector geomagnetic data from global magnetic observatories as well as the CHAMP and Swarm-A satellites (Ropp et al., 2020). To constrain the internal dynamics of the Earth’s core, we incorporated LOD data from the Earth Orientation Parameters series C04, provided by the International Earth Rotation and Reference Systems Service. The LOD dataset combines historical observations with modern space geodetic techniques including Very Long Baseline Interferometry, Satellite Laser Ranging, Global Navigation Satellite Systems and Lunar Laser Ranging, offering a continuous record from 1962 to present (Bizouard & Gambis, 2011).

After removing predictable tidal and atmospheric signals, LOD variations reflect exchanges of angular momentum between the Earth's core and mantle. Since electromagnetic waves such as torsional Alfvén waves generated in the Earth's core are linked to rapid geomagnetic accelerations, inclusion of LOD data may make a key constraint on the geomagnetic forecast. Our results show that a model trained only by geomagnetic secular acceleration (SA) failed to capture the 2014–2015 geomagnetic jerk, whereas adding LOD data showed an improved accuracy during the same event. Specifically, the SA misfit decreased from 4.98 to 2.43 nT/yr². The improvement was most significant when training with the second-order derivatives (i.e., SA snapshots themselves), indicating that the EKF-RNN successfully uncovered the underlying physical connection between geomagnetic acceleration and the Earth’s rotation. This study confirms that a multiple data approach, combining independent yet physically linked observation data, is essential for the next generation of geomagnetic forecast models.

How to cite: Toh, H., Sato, S., and Lesur, V.: Impact of Length-of-Day inclusion on geomagnetic secular variationforecast by a recurrent neural network, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15244, https://doi.org/10.5194/egusphere-egu26-15244, 2026.

EGU26-15271 | ECS | Orals | NP4.2

Storm-scale forecasting from observations 

Jaideep Pathak, Mohammad Shoaib Abbas, Peter Harrington, Zeyuan Hu, Noah Brenowitz, Suman Ravuri, Dale Durran, Corey Adams, Oliver Hennigh, Nicholas Geneva, Jussi Leinonen, Alberto Carpentieri, and Mike Pritchard

Accurate short-term prediction of clouds and precipitation is critical for severe weather warnings, aviation safety, and renewable energy operations. Traditional mesoscale numerical weather prediction models require significant modeling expertise and computational infrastructure. We introduce Stormscope, a family of transformer-based generative diffusion models trained directly on high-resolution, multi-band geostationary satellite imagery and ground-based radar over the Continental United States. Stormscope produces forecasts at a temporal resolution as high as 10 min and 6-km spatial resolution. Geostationary satellites and ground-based radar provide high-resolution, high-frequency observations essential for characterizing the evolving structure of the mesoscale atmosphere. Evaluated against extrapolation methods and operational mesoscale NWP models such as HRRR, Stormscope achieves leading performance on standard verification metrics including Fractions Skill Score and Continuous Ranked Probability Score across forecast horizons from 1 to 6 hours. By operating in native observation space, Stormscope establishes a new paradigm for AI-driven nowcasting with direct applicability to operational forecasting workflows. The approach is highly extensible, with demonstrated computational scaling to larger domains and higher resolutions. Critically, because Stormscope relies solely on globally ubiquitous satellite observations and radar where available, it offers a pathway to extend skillful mesoscale forecasting to oceanic regions and countries without existing strong operational mesoscale modeling programs.

How to cite: Pathak, J., Abbas, M. S., Harrington, P., Hu, Z., Brenowitz, N., Ravuri, S., Durran, D., Adams, C., Hennigh, O., Geneva, N., Leinonen, J., Carpentieri, A., and Pritchard, M.: Storm-scale forecasting from observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15271, https://doi.org/10.5194/egusphere-egu26-15271, 2026.

EGU26-16098 | ECS | Orals | NP4.2

CondensNet: Self-adaptive physical constraints for stable long-term hybrid climate simulations 

Xin Wang, Gianmarco Mengaldo, Jianda Chen, Juntao Yang, Jeff Adie, Simon See, Kalli Furtado, Chen Chen, Troy Arcomano, Romit Maulik, and Wei Xue
Accurate and efficient climate simulations are crucial for understanding Earth’s evolving climate. However, current General Circulation Models (GCMs) face challenges in capturing unresolved physical processes, such as cloud and convection. A common solution is to adopt Cloud-Resolving Models (CRMs), which provide more accurate results than the standard subgrid parameterization schemes typically used in GCMs. However, CRMs (also referred to as super-parameterizations, such as SPCAM) remain computationally prohibitive. Hybrid modeling, which integrates deep learning with equation-based GCMs, offers a promising alternative but often struggles with long-term stability and accuracy issues.
 
In this work, we find that water vapor oversaturation during condensation is a key factor compromising the stability of hybrid modeling. To address this, we introduce CondensNet, a novel neural network architecture that embeds a self-adaptive physical constraint to correct unphysical condensation processes. CondensNet effectively mitigates water vapor oversaturation, enhancing simulation stability while maintaining accuracy and improving computational efficiency compared to super-parameterization schemes.
 
We integrate CondensNet into a GCM to form PCNN-GCM (Physics-Constrained Neural Network GCM), a hybrid deep learning framework designed for long-term stable climate simulations under real-world conditions (AMIP setting). PCNN-GCM enables stable simulations over decades and achieves up to 370× speed-up compared with SPCAM, while also being faster than traditional CAM5 under GPU acceleration or CPU-only. Beyond stability and efficiency, PCNN-GCM demonstrates greater skill in capturing complex climate variability than CAM5, including tropical precipitation extremes and the Madden-Julian Oscillation (MJO), yielding results that align more closely with observations or reanalyses (e.g., ERA5, TRMM) than conventional parameterization schemes.

How to cite: Wang, X., Mengaldo, G., Chen, J., Yang, J., Adie, J., See, S., Furtado, K., Chen, C., Arcomano, T., Maulik, R., and Xue, W.: CondensNet: Self-adaptive physical constraints for stable long-term hybrid climate simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16098, https://doi.org/10.5194/egusphere-egu26-16098, 2026.

EGU26-16240 | Posters on site | NP4.2

Inductive Biases for Robust Climate Emulation Across Forecast Timescales 

Oskar Bohn Lassen, Francisco Camara Pereira, Simon Driscoll, Sebastian Schemm, and Stephen Thomson

Machine-learning emulators have demonstrated remarkable skill for weather prediction and short-range forecasting, yet their behaviour, as forecasts extend toward seasonal and longer timescales, remains less well explored and understood. Approaching these horizons, forecast skill is shaped less by short-range error growth, while variations in background states or system parameters increasingly influence the evolving dynamics. Understanding if and how different neural architectures perform with such changes is therefore central to assessing their suitability for emulation beyond medium range weather prediction, where robustness plays an increasingly important role. In this work, we investigate how inductive biases encoded in deep-learning architectures influence their ability to represent and evolve dynamics as forecasts move into windows nearing and sometimes beyond their training data.

We use the idealised climate model ISCA as a controlled testbed, enabling systematic variation of planetary parameters and initial conditions while retaining a fixed underlying set of governing equations. Emulators are trained on ensembles of trajectories sampled from a restricted parameter range and evaluated under progressively more challenging ID/OOD settings. This framework allows us to disentangle errors arising from finite-horizon forecasting from those associated with longer-timescale dynamical shifts, providing insight into which architectural biases promote stability, physical consistency, and robustness as machine-learning models are pushed from shorter term prediction toward longer time scale emulations.

How to cite: Bohn Lassen, O., Camara Pereira, F., Driscoll, S., Schemm, S., and Thomson, S.: Inductive Biases for Robust Climate Emulation Across Forecast Timescales, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16240, https://doi.org/10.5194/egusphere-egu26-16240, 2026.

EGU26-16454 | ECS | Orals | NP4.2

Emulating climate variability and extremes with a multivariate flow matching model trained on CESM2 and finetuned on ERA5 

Violette Launeau, Mathieu Vrac, Léo Lemordant, and Pierre Gentine

In the context of increasing interest in machine learning-based emulators to overcome the computational cost and limited scenario coverage of Earth System Models (ESMs), some key challenges remain, such as capturing internal variability, handling non-stationarity, and realistically representing compound and extreme events — especially at high spatial and temporal resolution.

We present a probabilistic multivariate emulator of climate variables based on a flow matching model trained on the CESM2 Large Ensemble (Danabasoglu et al., 2020) under the SSP3-7.0 scenario. Our approach leverages a flow matching framework (Lipman et al., 2022) to reproduce the spatiotemporal variability of temperature and precipitations on a monthly timescale. The model is conditioned on greenhouse gas concentrations and we evaluate the capability of the model  to generate physically consistent climate fields and to capture the full ensemble spread of the original ESM, including tail behavior and potential extreme events. To ensure a better reproduction of observed climatological variability, the flow matching model is fine-tuned on ERA5 reanalyses (Hersbach et al., 2020). This should enable the emulator to act as a stochastic weather generator of plausible climate states under GHG forcing trajectories, accounting for the non-stationarity introduced by anthropogenic climate change, and allowing for the assessment of rare or compound extreme events within the generated ensemble. Our results assess the model’s ability to reproduce ensemble-scale statistics, cross-variable dependencies, and evolving climate distributions across time. 

How to cite: Launeau, V., Vrac, M., Lemordant, L., and Gentine, P.: Emulating climate variability and extremes with a multivariate flow matching model trained on CESM2 and finetuned on ERA5, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16454, https://doi.org/10.5194/egusphere-egu26-16454, 2026.

EGU26-18204 | ECS | Orals | NP4.2

Coupling ICON with a Machine Learning Emulator for Cloud Microphsysics 

Paul Keil, Caroline Arnold, and Shivani Sharma

As the spatial resolution of general circulation models (GCMs) increases and storms and clouds can be resolved, the underlying cloud microphysics still need to be parameterised. This is known to be a major source of uncertainty in climate and weather simulations. The established parameterisations use bulk moment schemes, where the conversion of cloud and rain droplets is approximated through empirical relationships. Particle-based superdroplet simulations would provide a more accurate representation but are typically not feasible for use in GCMs.

We couple SuperdropNet, an ML emulator for warm rain cloud microphysics trained on superdroplet simulations, to ICON. Previously, we validated the coupled model in an idealised cloud microphysics test case and showed that SuperdropNet runs stable and provides reasonable precipitation patterns.

Now we move towards a climate model experiment with 10 km horizontal resolution in an AMIP setup to investigate SuperdropNet’s feasibility and interaction with ICON in a realistic setting. Coupling SuperdropNet to ICON is achieved using FTorch. We are able to run ICON on 128 nodes on the CPU partition of the HPC system Levante with minimal overhead. Conditions beyond the training data range of SuperdropNet lead to negative feedback loops and impact the long-term stability of the coupled simulation. Therefore, we implement physics-based constraints that improve stability. Initial results show mean surface precipitation is very similar to using the bulk scheme approach. SuperdropNet simulates a faster cloud-to-rain transition which impacts cloud water mass and rain droplet size. This has consequences for the radiation budget and the frequency distribution of precipitation. Furthermore, we show that an autoregressive rollout of SuperdropNet that allows for longer GCM time steps runs stable and does not impact results. Finally, we test SuperdropNET’s generalisation capabilities in a 4K warmer world.

How to cite: Keil, P., Arnold, C., and Sharma, S.: Coupling ICON with a Machine Learning Emulator for Cloud Microphsysics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18204, https://doi.org/10.5194/egusphere-egu26-18204, 2026.

EGU26-18659 | ECS | Orals | NP4.2

Hierarchical Graph Networks for ForecastingTerrestrial Water Storage Anomalies 

Viola Steidl and Xiao Xiang Zhu

The availability of fresh water is vital to the ecosystem and communities. In a changing climate, the increased risk of droughts makes it crucial to have an accurate understanding of changes in terrestrial water storage (TWS). Predicting changes in TWS is inherently difficult since it integrates the changes of all water compartments, with underlying processes that operate on vastly different temporal and spatial scales. 

Forecasting tasks nowadays are often solved using machine learning models. However, these models require vast amounts of data. In contrast, total water storage anomalies (TWSA) derived from GRACE/GRACE-FO observations only date back to 2002 and are available at a grid of 1°x1° at monthly resolution. Nevertheless, Li et al., (2024) showed that machine-learning approaches could forecast TWSA tendencies for up to one year ahead. They cleverly exploit temporal lag relationships between TWSA and ocean, atmospheric, or land variables.

In our work, we explore a novel design of a hierarchical graph using domain knowledge of hydrological basins to encode these processes in a latent feature sequence using an encoder-processor-decoder style graph neural network. The subsequent recurrent neural network then forecasts TWSA from the latent feature sequence and 12-month history of TWSA for up to six months ahead. The gridded product of the seasonal forecast of global TWSA shows improvement over a seasonal long-term mean.

Li, F., Kusche, J., Sneeuw, N., Siebert, S., Gerdener, H., Wang, Z., Chao, N., Chen, G., and Tian, K.: Forecasting Next Year’s Global Land Water Storage Using GRACE Data, Geophys. Res. Lett., 51, e2024GL109101, https://doi.org/10.1029/2024GL109101, 2024.

How to cite: Steidl, V. and Zhu, X. X.: Hierarchical Graph Networks for ForecastingTerrestrial Water Storage Anomalies, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18659, https://doi.org/10.5194/egusphere-egu26-18659, 2026.

EGU26-19872 | Posters on site | NP4.2

Extending foundation models from weather to climate: challenges and promises 

Fanny Lehmann, Riccardo Neumarker, Gabriele Scorrano, Yun Cheng, Salman Mohebi, Firat Ozdemir, Junyang Gou, Oliver Fuhrer, Torsten Hoefler, Siddhartha Mishra, Mathieu Salzmann, Sebastian Schemm, and Benedikt Soja

AI weather models and weather-based foundation models have demonstrated impressive skills in short- to medium-range forecasts. While most weather models become unstable on longer time scales, a wide variety of AI climate emulators have been proposed, raising questions about the fundamental differences between these approaches.

In this work, we compare state-of-the-art models when producing rollouts on annual time scales. We quantify and characterize different types of instability: smoothing, visual artifacts, drift, and loss of seasonality. This analysis highlights the previously unreported stability of the Aurora foundation model and the Earth System Foundation Model (ESFM) for rollouts longer than 35 years.

To encompass more diverse representations of possible states of the Earth, ESFM is pretrained on a variety of CMIP6 datasets from the historical period, in addition to the ERA5 reanalysis commonly used in AI models. ESFM also includes climate forcings for physically driven long rollouts. We demonstrate the benefits of CMIP6 pretraining when finetuning on new CMIP6 datasets, including datasets with higher resolution, unseen physical processes, and climate change scenarios.

Overall, this work opens perspectives to adapt large-scale pretrained foundation models to the specific challenges of climate projections.

How to cite: Lehmann, F., Neumarker, R., Scorrano, G., Cheng, Y., Mohebi, S., Ozdemir, F., Gou, J., Fuhrer, O., Hoefler, T., Mishra, S., Salzmann, M., Schemm, S., and Soja, B.: Extending foundation models from weather to climate: challenges and promises, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19872, https://doi.org/10.5194/egusphere-egu26-19872, 2026.

EGU26-20131 | Orals | NP4.2

Solving the lack of data issue for machine learning for rare climate events 

Amaury Lancelin, Freddy Bouchet, Alexander Wikner, Pedram Hassanzadeh, Laurent Dubus, and Peter Werner

Machine learning is reshaping the entire climate-modelling chain, from climate model development to the study of climate extreme events and their impacts. One of the key drivers of this revolution is the availability of datasets that are sufficiently large for training and validation. For climate extreme events, however, this requirement poses seemingly insurmountable challenges: we need to assess the impacts of unprecedented events for which historical data are too scarce; we must rely on models, yet simulating extremely rare events with them is prohibitively expensive; and any statistical approach, including machine learning, suffers from a severe lack-of-data problem.

Here, we argue that the only viable path forward is to integrate machine learning directly into the data-generation process, in close interaction with state-of-the-art physics-based climate models and observational datasets.

The first building block of our approach is the development of state-of-the-art climate model emulators. AI models trained on historical reanalyses to emulate the dynamics of the global atmosphere have demonstrated both high forecast skill and drastically reduced computational costs. Some of these AI emulators can generate stable trajectories spanning multiple decades, which, combined with their affordability, has the potential to significantly reduce uncertainties related to extreme weather. However, it remains impossible to directly validate whether AI emulators can reliably estimate the risk of extreme events with return times exceeding the historical record. To address this issue, we develop a methodology based on state-of-the-art architectures, with the explicit requirement that emulators exhibit extremely long-term stability, high fidelity, and a faithful reproduction of the stationary statistics of the climate model.

In a first-of-its-kind experiment, we simulate 100,000 years of a stationary climate using PlaSim, a coarse-resolution general circulation model. We then train a set of stable AI emulators using only 100 years of data, and compare the return times of extreme heat waves over Western Europe and the Pacific Northwest, as well as severe precipitation events over the Tropics.

The second building block of our approach consists of rare-event simulation techniques that reduce by several orders of magnitude the computational cost of sampling extremely rare events with CMIP-class climate models. The third building block is the blending of historical observations with CMIP model output within a Bayesian framework to estimate the

probability of extremely rare events constrained by observations. In this talk, we also briefly discuss the second and third building blocks and their connections to the first within a comprehensive, integrated framework.

How to cite: Lancelin, A., Bouchet, F., Wikner, A., Hassanzadeh, P., Dubus, L., and Werner, P.: Solving the lack of data issue for machine learning for rare climate events, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20131, https://doi.org/10.5194/egusphere-egu26-20131, 2026.

EGU26-21143 | Posters on site | NP4.2

Weather and Climate: Applications of Machine Learning and Artificial Intelligence 

Simon Driscoll, Kieran Hunt, Laura Mansfield, Ranjini Swaminathan, Hong Wei, Eviatar Bach, and Alison Peard

We demonstrate software and tools for users to progress from machine learning theory, probabilistic methods, through to construction of AI models across environmental science. We span basic AI methods through to modern generative AI methods, physics informed techniques, as well as including a vast array of concrete applications such as river discharge modelling, ocean-wave emulation, environmental monitoring, AI foreasting and more. Throughout we place emphasis on how and when these methods should be used, as well as their limitations. This allows users to develop a non-naive understanding of AI and to engage with all themes of Machine Learning Across Earth System Modeling: Subgrid-Scale Parameterizations, Emulation and Hybrid Modeling.

How to cite: Driscoll, S., Hunt, K., Mansfield, L., Swaminathan, R., Wei, H., Bach, E., and Peard, A.: Weather and Climate: Applications of Machine Learning and Artificial Intelligence, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21143, https://doi.org/10.5194/egusphere-egu26-21143, 2026.

EGU26-21279 | ECS | Posters on site | NP4.2

Geometry- and Physics-Aware Dataset Creation for Shadow Removal in High-Resolution Satellite Imagery 

Lorenzo Beltrame, Jules Salzinger, Phillipp Fanta-Jende, Jasmin Lampert, Pascal Leon Thiele, Filip Svoboda, Radu Timofte, and Marco Körner

Shadows cast by terrain and tall structures are a persistent limitation in satellite imagery, since they degrade radiometric consistency and compromise downstream tasks such as classification, detection, and 3D reconstruction. In this context, machine learning methods for shadow removal provide a flexible and easy-to-deploy tool to assist satellite remote sensing tasks.  Nevertheless, one prominent issue for its development in Earth Observation (EO) is the scarcity of publicly available, geometry-consistent paired shadowed/shadow-free satellite data. Most EO resources support shadow detection or 3D modelling but not shadow removal, while existing shadow-removal datasets largely target ground-level or UAV imagery and do not reflect multi-date, multi-angle satellite acquisition.

To address this gap, we present deSEO, a physics-informed, geometry-aware methodology that converts anyinto paired training data for weakly supervised satellite shadow removal. We exemplified our procedure on the S-EO satellite dataset. Using the multi-temporal, multi-geometry S-EO dataset (WorldView-3 imagery with DSM priors, simulated shadow masks, and RPC camera models), deSEO selects a minimally shadowed acquisition per tile as a proxy reference and pairs it with more shadowed dates under explicit temporal and geometric constraints. Residual off-nadir parallax is mitigated through orientation normalisation and feature-based registration (LoFTR + RANSAC), yielding a per-pixel validity mask that can be used to restrict model supervision to reliably aligned regions.

To validate the usability of the shadow-removal dataset derived from S-EO, we first adapted UAV-oriented methods such as SRNet and pix2pix. However, these approaches fail to converge to a stable training regime under the viewpoint variability typical of satellite acquisitions. We therefore develop a more robust method and training strategy that mitigates this common failure mode of image-to-image translation on multi-date, multi-geometry satellite imagery. Our approach involves training a DSM-conditioned conditional GAN with a U-Net-based generator. The model incorporates perceptual reconstruction and mask-constrained adversarial objectives, with a soft shadow-mask attention prior that emphasises shadow-transition regions. These enhancements overcome the limitations of the classical GAN image translation setup that worked well for UAV data. We evaluate the model on a held-out test split, where the proposed approach achieves a PSNR of 18 ± 1 dB, SSIM of 0.49 ± 0.08, and LPIPS of 0.46 ± 0.05. Notably, improvements were most pronounced at cast-shadow boundaries, and ablation studies revealed that DSM conditioning was the dominant contributing factor, something absent in the SRNet model.

Overall, deSEO provides a reproducible approach to derive paired supervision for satellite shadow removal and establishes a geometry-aware baseline for robust deshadowing under realistic EO acquisition variability.

How to cite: Beltrame, L., Salzinger, J., Fanta-Jende, P., Lampert, J., Thiele, P. L., Svoboda, F., Timofte, R., and Körner, M.: Geometry- and Physics-Aware Dataset Creation for Shadow Removal in High-Resolution Satellite Imagery, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21279, https://doi.org/10.5194/egusphere-egu26-21279, 2026.

EGU26-21434 | ECS | Orals | NP4.2

Quantum-inspired machine learning for efficient and reliable weather forecasting  

Osama Ahmed, Sallar Ali Qazi, and Luca Magri

Recent advances in data-driven weather forecasting have demonstrated skill at medium-range lead times, yet often rely on extremely large models, massive training datasets, and substantial computational resources. In this talk, we present a novel quantum-inspired machine learning (QIML) approach for sub-seasonal weather forecasting that prioritizes computational efficiency and dynamical stability, while retaining competitive predictive skill.

First, by using quantum circuits ansätze and entanglement, we design scalable quantum reservoir computing models. The implemented model is parallelizable across multiple GPUs and runs on classical hardware in a quantum-inspired setting. Second, we train our model on ERA-5 reanalysis data for 2m temperature, multiple pressure levels, and precipitation on a global grid. We show that, using an encoder-decoder architecture in conjunction with the proposed QIML model, we demonstrate forecasts of key atmospheric variables up to 45 days ahead. Third, we benchmark our model against state-of-the-art AI for weather forecasting methods and show that the QIML model can produce reliable forecasts for weather and climate extremes, while requiring 10-50X less compute.  Fourth, replacing conventional neural architectures with quantum-inspired circuit dynamics enables enhanced physical interpretability and consistency, as the model state evolves according to Schrödinger-type dynamics. We further analyze the learned latent representations using operator-theoretic and spectral tools, revealing coherent structures associated with dominant atmospheric modes.

This work proposed a novel direction to the growing ecosystem of hybrid ML physics approaches by offering a new class of lightweight, stable, and scalable forecasting models that can be deployed efficiently for localized and resource-constrained settings. 

How to cite: Ahmed, O., Qazi, S. A., and Magri, L.: Quantum-inspired machine learning for efficient and reliable weather forecasting , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21434, https://doi.org/10.5194/egusphere-egu26-21434, 2026.

EGU26-22145 | ECS | Orals | NP4.2

Seamless Storm Surge Prediction Using a Surrogate Hydrodynamic Model Based on Long Short-Term Memory Networks 

Villy Mik-Meyer, Francisco C. Pereira, Morten Andreas Dahl Larsen, Jian Su, and Martin Drews

Accurate storm surge prediction is essential for reducing the risks associated with extreme sea levels and for supporting early warning and preventive measures. Physically based numerical models continue to improve in skill and resolution, but their high computational cost limits their use in large ensembles and long-term scenario analyses. Recent advances in machine learning offer a complementary pathway for efficient storm surge forecasting. Here, a machine-learning framework is developed, calibrated, and validated to predict extreme sea levels in the North Sea and Baltic Sea. The model is based on 58 years of spatially distributed wind data and uses a Long Short-Term Memory (LSTM) architecture to capture the temporal dynamics driving water level variability. Compared to traditional physically based hydrodynamic models, the machine-learning approach requires only a fraction of the computational resources, enabling rapid probabilistic and large-ensemble forecasts across large domains and extended time periods. This efficiency is particularly valuable for climate change research, where large ensembles are generally needed to address the combined uncertainty of climate and hydrodynamic models but remain computationally prohibitive using conventional approaches. By providing a scalable and resource-efficient alternative, this framework enables consistent storm surge prediction across timescales ranging from short-term forecasting to long-term climate projections over decades.

How to cite: Mik-Meyer, V., Pereira, F. C., Larsen, M. A. D., Su, J., and Drews, M.: Seamless Storm Surge Prediction Using a Surrogate Hydrodynamic Model Based on Long Short-Term Memory Networks, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22145, https://doi.org/10.5194/egusphere-egu26-22145, 2026.

EGU26-22628 | ECS | Posters on site | NP4.2

A Comparative Evaluation of Grid-Invariant Deep Learning Surrogate Models for Wildfire Simulation 

Matheu Boucher, Jidan Zhang, Christopher Pain, Yueyan Li, Aniket Joshi, Ben Moseley, and Philip Cunningham

As climate change drives more extreme wildfire behavior, accurate and computationally efficient fire spread modeling is increasingly critical for monitoring, mitigation, and risk assessment. Wildfires pose a particularly challenging modeling problem due to their complex interactions with fuels, terrain, and atmospheric conditions, as well as their potential to impact populated regions with severe environmental, economic, and human consequences. These challenges motivate the development of surrogate modeling approaches capable of emulating physics-based wildfire simulations at substantially reduced computational cost. In this work, we present a systematic comparison of two deep learning surrogate model architectures for spatiotemporal wildfire emulation: a convolutional neural network-based generative model and a conditional diffusion model. Both approaches are designed to be grid-invariant and trained to predict three key wildfire variables – time of arrival, flame length, and burn scar – at fixed 15-minute time steps. Model performance is evaluated using an autoregressive rollout procedure in which successive short-term predictions are recursively fed back as inputs to simulate wildfire evolution over 12-hour time horizons. The training data consists of wildfire simulations generated using a Rothermel-based fire spread model with realistic, satellite-derived fuel distributions over the western United States (California and Nevada). Evaluation is performed on geographically distinct fire scenarios to assess generalization across diverse fuel configurations. Both surrogate models are shown to produce stable and physically plausible wildfire dynamics over 12-hour autoregressive rollouts while reducing inference time relative to physics-based solvers. The results highlight the potential of deep generative surrogates to enable rapid ensemble-based risk assessment and support operational fire management workflows under diverse environmental conditions.

How to cite: Boucher, M., Zhang, J., Pain, C., Li, Y., Joshi, A., Moseley, B., and Cunningham, P.: A Comparative Evaluation of Grid-Invariant Deep Learning Surrogate Models for Wildfire Simulation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22628, https://doi.org/10.5194/egusphere-egu26-22628, 2026.

EGU26-6596 | ECS | Orals | NP4.4

Recurrence Lacunarity for the Analysis of Spatial Data 

Cara Bielig, Aljoscha Rheinwalt, Tobias Braun, and Norbert Marwan

Quantifying the structure and heterogeneity of complex spatial patterns is a key challenge in the analysis of spatial data across many scientific disciplines, including geoscience and geomorphology. The complexity of spatial patterns can be analysed by considering the recurrence of specific properties. While recurrence plot based methods are well established for analysing dynamical systems, their application to spatial patterns has received less attention. Here, we propose a novel approach that combines spatial recurrence analysis with a measure from fractal geometry, lacunarity, which originally quantifies homogeneity in spatial patterns. Applied to recurrence plots, it is referred to as recurrence lacunarity (RL) and quantifies the homogeneity of recurrences. Although recurrence plots can be generated from higher-dimensional data, RL has not yet been calculated for higher-dimensional (spatial) recurrence plots. To address this gap, we evaluate the RL of spatial data by validating the method using synthetic test patterns and then applying it to analyse hillslope gradients of river catchments near the Mendocino Triple Junction. The results demonstrate that the RL effectively detects and quantifies differences in the spatial structure of the catchments, which can be related to local uplift rates and the geological setting. RL provides a robust measure for comparing diverse spatial data sets and for quantifying how their spatial structure relates to external parameters, and may also be used as features in machine-learning models, complementing existing descriptors of spatial structure.

How to cite: Bielig, C., Rheinwalt, A., Braun, T., and Marwan, N.: Recurrence Lacunarity for the Analysis of Spatial Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6596, https://doi.org/10.5194/egusphere-egu26-6596, 2026.

EGU26-6824 | ECS | Posters on site | NP4.4

Detecting Climate Transitions with Recurrence Plots: A Case Study of the Younger Dryas 

Zinan Lyu, Dirk Sachse, Norbert Marwan, and Hui Tang

Identifying regime shifts in paleoclimate proxy records remains challenging when time series are short and irregularly sampled. Such characteristics are common in paleoclimate archives and often limit the applicability of traditional linear statistical methods for quantifying regime transitions. In this study, we focus on the Younger Dryas event using a unique, biomarker stable isotope-based paleoclimate proxy dataset derived from two distinct lake sediment records that were hydrologically connected in the paleoenvironment. The proxy signals from both sediment cores exhibit strong similarities but also notable differences. We therefore use them as a ‘replicate’ sample, providing a natural framework for comparative analysis.

Recurrence plots and recurrence quantification analysis are employed to characterize nonlinear variability and to compare structural patterns between the two records. The recurrence plots capture the overall temporal extent of the Younger Dryas event in both proxies, while revealing small offsets in its onset and termination. These differences suggest potential influence of local environmental conditions on the lake systems and provide additional insights into site-specific responses. By analyzing the residual differences between the two proxy records, smaller-scale features can be identified, potentially reflecting local processes hidden by the large-scale climatic signal.

 

How to cite: Lyu, Z., Sachse, D., Marwan, N., and Tang, H.: Detecting Climate Transitions with Recurrence Plots: A Case Study of the Younger Dryas, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6824, https://doi.org/10.5194/egusphere-egu26-6824, 2026.

EGU26-7598 | Orals | NP4.4

Evaluation of streamflow complexity of two major Indian river basins using dynamic recurrence theoretical approach 

Adarsh Sankaran, Hudha Hameed Cheriyalicheth, and Shadiya Athayakkoth

This study presents dynamic application of recurrence quantification analysis (RQA) as an alternative approach for evaluation of streamflow complexity. Daily streamflows of 67 stations positioned in two major basins namely Mahanadi and Cauvery located at northern and southern India for 1980-2020 period are considered for recurrence analysis  (RA). Then a novel dynamic recurrence theory (DRT) approach is followed for evaluating the complexity of multiple streamflow segments along the time domain. The key recurrence measures such as Determinism, Laminarity, Entropy, Trapping Time along with mean diagonal length are quantified for multiple  segments along the temporal domain. The temporal evolution of recurrence measures showed abrupt alternations in complexity measures in majority of stations, except for 6 stations (16 %) of Mahanadi and 5 stations (17 %) of Cauvery, mostly falling within 1985-2000 period. The drastic shifts in complexity measures are coinciding more with the anthropogenic impacts than climatic drivers. The streamflow dynamics of  Cauvery basin is found to be more erratic and complex than that of Mahanadi basin. In general, the streamflow dynamics of stations located in lower reaches are more complex and controlled by flow regulations than that of the upper reaches of both the basins. The insights gained from the novel DTA approach are noted to be helpful in identifying the prominent changes in streamflow and hence giving better insights on to its predictability.

 

How to cite: Sankaran, A., Cheriyalicheth, H. H., and Athayakkoth, S.: Evaluation of streamflow complexity of two major Indian river basins using dynamic recurrence theoretical approach, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7598, https://doi.org/10.5194/egusphere-egu26-7598, 2026.

EGU26-7745 | ECS | Posters on site | NP4.4

Nonlinearity of teleconnections in paleoclimatological data 

Petr Skala

Teleconnections in the climate system are a central element of internal variability, yet their degree of nonlinearity and long-term properties remain largely unexplored, especially in a paleoclimatological context. In our investigation, we perform a statistical analysis on data from the ModE-RA paleo-reanalysis to assess the spatial structure and nonlinear character of major atmospheric teleconnections over the last five centuries. We employ the mutual information measure, combined with surrogate data methods to detect statistically significant nonlinearities in the two-dimensional system formed by gridded temperature time series and indices of major modes of internal variability. This approach allows us to identify behaviour which may not be captured by linear correlation methods. Attention is also paid to the possibility of regime shifts or changes in large-scale forcings across different periods.

How to cite: Skala, P.: Nonlinearity of teleconnections in paleoclimatological data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7745, https://doi.org/10.5194/egusphere-egu26-7745, 2026.

EGU26-8889 | ECS | Orals | NP4.4

Recurrence networks-based analysis of soil moisture dynamics in global land areas 

Anagha Prabhakar and Bellie Sivakumar

Soil moisture is a complex nonlinear hydroclimatic variable playing a significant role in the hydrologic cycle. Soil moisture has great influence on land-atmospheric interactions, including triggering and shaping extreme events, especially under climate change. Therefore, identifying hidden patterns and structures in soil moisture dynamics and understanding their evolution are critical for a wide range of applications. In this study, we aim to explore the temporal dynamics of soil moisture systems across global land areas using recurrence network analysis, bridging complex networks concept and recurrence plots. We use GLDAS soil moisture data in global land areas for 1948–2024 at a spatial resolution of 1 degree x 1 degree. Recurrence networks of soil moisture systems are constructed from soil moisture time series at individual grids. The nodes of the network represent the states of the system, and the links represent the recurrence of states. The nodes of the recurrence networks are identified by delay embedding of the soil moisture time series (i.e., phase space reconstruction) in an optimum embedding dimension identified using the False Nearest Neighbour algorithm. Thereafter, the links of the networks are established by considering the closeness of the nodes in terms of Euclidean distances. Several complex network measures, such as degree centrality, betweenness centrality, shortest path length, and clustering coefficient, are used to interpret the soil moisture systems from a recurrence perspective. The results from this study suggest that the soil moisture system behavior is similar for regions characterized with similar precipitation regime. This understanding is highly relevant for identifying regions with similar land-atmospheric coupling processes.

How to cite: Prabhakar, A. and Sivakumar, B.: Recurrence networks-based analysis of soil moisture dynamics in global land areas, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8889, https://doi.org/10.5194/egusphere-egu26-8889, 2026.

EGU26-9506 | ECS | Posters on site | NP4.4

Recurrence Analysis of Communities from Precipitation Patterns over the Indian Peninsula 

Mia Janzen, Sree Anusha Ganapathiraju, and Norbert Marwan

Precipitation is a crucial component of the hydrological cycle and is essential for water supply, ecosystems, and climate dynamics. 
In this context, the monsoon-driven rainfall patterns of the Indian Peninsular (IP) region exhibit a distinct spatio-temporal variability due to its strong seasonality, complex topography, and regional heterogeneity. Consequently, a key challenge is to identify local rainfall regimes and assess how their temporal evolution and recurrence patterns vary across space and seasons.
To address this, we leverage the recurrence analysis framework to comprehend the non-linear rainfall dynamics in terms of their deterministic behavior. 
We apply singular value decomposition and agglomerative hierarchical clustering to extract spatial communities with similar recurrence characteristics. In addition, Laplacian centrality is used to determine central hubs within each community. Furthermore, to analyze long-term trends in predictability and  persistence of rainfall dynamics, we employ a bootstrapping framework based on recurrence quantification analysis measures, comparing periods before and after 1991. 
The study uncovers four communities within the IP region, which are generally shifting towards less predictable dynamics over time. The overall cluster organization varies substantially in terms of season and time period, while the spatial locations of the central hubs within each community remain stable. In particular, the community located in the western region exhibits a pronounced decline in recurrence.
In summary, these findings indicate that rainfall dynamics in the IP region is undergoing both a temporal shift towards reduced predictability and a spatial reorganization. The study exemplifies the applicability of recurrence analysis to characterize the intrinsic nonlinear dynamics of the climate system, detect regime transitions, and provide insights that support disaster preparedness and adaptation planning.

How to cite: Janzen, M., Ganapathiraju, S. A., and Marwan, N.: Recurrence Analysis of Communities from Precipitation Patterns over the Indian Peninsula, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9506, https://doi.org/10.5194/egusphere-egu26-9506, 2026.

EGU26-9520 | Orals | NP4.4

Leveraging Real-Time Stochasticity to Detect Transient States in Complex Systems 

Pouya Manshour, M. Reza Rahimitabar, and Milan Paluš

Detecting transient states and critical transitions in complex systems is essential for predicting abrupt shifts in phenomena such as climate stability, biological health, and financial market trends. However, identifying these transitions in real-time is particularly challenging in noisy, non-stationary data. To address this, we introduce stochasticity, defined as the square of short-term fluctuations within a sliding time window dt [1], as a time-resolved metric for capturing system instability. We demonstrate that stochasticity can serve as a highly sensitive indicator of emerging transient phases, and show that it converges more accurately than traditional drift-based measurements. This approach can identify transitions in diverse domains, including regional temperature anomalies and Parkinson’s disease progression via keystroke dynamics and thus provides a robust tool for monitoring systems where traditional methods struggle to resolve rapid changes.

This project was supported by the Czech Science Foundation, Project No. 25-18105S.

[1] Rahvar, Sepehr, et al. "Characterizing time-resolved stochasticity in non-stationary time series." Chaos, Solitons & Fractals 185 (2024): 115069.

How to cite: Manshour, P., Rahimitabar, M. R., and Paluš, M.: Leveraging Real-Time Stochasticity to Detect Transient States in Complex Systems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9520, https://doi.org/10.5194/egusphere-egu26-9520, 2026.

EGU26-11122 | Posters on site | NP4.4

Comparing deterministic and stochastic methods to infer causal Earth system interactions 

Niclas Schilling, Ingo Fetzer, Kira Rehfeld, and Hannah Zoller

In an era often referred to as 'the Great Acceleration', it is becoming increasingly urgent to identify causal structures in intertwined Earth system processes. This has led to the development of a wide range of causal inference methods that aim to accurately distinguish causal influences from pure correlation. Many of the established tools fall within two methodological families: state-space approaches, which reconstruct deterministic dynamics, and information-theoretic approaches, which are formulated for coupled stochastic processes. Despite their widespread use, clear guidance on the conditions under which these different approaches are appropriate, and on the associated trade-offs, remains fragmented.

Here, we present a systematic comparison of two representatives from these methodologically different backgrounds. We focus on convergent cross mapping, a deterministic approach, and transfer entropy, a stochastic approach. Both are commonly used for identifying and quantifying interactions in the Earth system from time series data. We assess their performance using (i) synthetic coupled systems with a known causal structure and (ii) real-world meteorological data on the Walker circulation, for which there exists an established physical understanding that can be used as a benchmark. Furthermore, we evaluate the impact of typical challenges related to the data (e.g. observation length, noise) and the underlying dynamics (e.g. latent drivers, causal delay) on detection ability and reliability, and test the sensitivity of the results to initial configuration choices.

Through this work, our aim is to provide a practical workflow and a set of recommendations that clarify the strengths, limitations, and potential synergies of these two conceptually distinct approaches. Finally, we outline and discuss potential use cases in current Earth system research.

How to cite: Schilling, N., Fetzer, I., Rehfeld, K., and Zoller, H.: Comparing deterministic and stochastic methods to infer causal Earth system interactions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11122, https://doi.org/10.5194/egusphere-egu26-11122, 2026.

Large-scale climate oscillations influence agricultural drought by altering atmospheric circulation, moisture transport, and land–atmosphere interactions. Understanding how climate oscillations organize the spatial connectivity of agricultural drought across different time lags remains a key challenge for regional drought assessment and predictability. To address this challenge, this study investigates the lag-dependent spatial connectivity between major climate oscillations and agricultural drought using an event-based complex network framework. For implementation, agricultural droughts in India are studied. Drought events are identified using a standardized soil moisture index for the period 1951–2014. Using these identified drought events, Event Coincidence Analysis is first applied to identify statistically significant lagged relationships between drought occurrence and the phases of major climate oscillations, including the El Niño–Southern Oscillation (ENSO), Indian Ocean Dipole (IOD), Pacific Decadal Oscillation (PDO), Atlantic Multidecadal Oscillation (AMO), and North Atlantic Oscillation (NAO), across multiple lead times (τ = 1, 3, 6, 9, and 12 months). Subsequently, these lag-specific relationships are used to construct complex networks that explicitly represent spatial connections between climate oscillations and drought events. The network analysis reveals clear and systematic regional patterns. Arid, semi-arid, and sub-humid regions consistently exhibit high network degree values, indicating strong connectivity with multiple climate oscillations, particularly at short to intermediate time lags. This suggests that droughts in these regions are driven by compound climate influences originating from different ocean basins. In contrast, humid regions display lower network degree values across all time lags, indicating weaker sensitivity to large-scale climate variability. Overall, the results demonstrate that agricultural drought across India is governed by lag-dependent and spatially organized climate influences rather than by a single dominant climate driver. The proposed framework provides a direct link between temporal climate signals and spatial drought connectivity, offering a robust basis for improving drought monitoring and early warning systems.

 

How to cite: Venkatesh, K. and Sivakumar, B.: Exploring Lag-Dependent Spatial Connectivity Between Climate Oscillations and Agricultural Drought: A Complex Network Approach, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14332, https://doi.org/10.5194/egusphere-egu26-14332, 2026.

EGU26-14733 | Posters on site | NP4.4

A new two-dimensional extension of the generalized Higuchi estimator for multifractal data: Theory and application to geoscience problems 

Carlos Carrizales-Velazquez, Lev Guzmán-Vargas, and Reik V. Donner

In 1988, Tomoyuki Higuchi introduced an algorithmic approximation of the box-counting dimension of the graph of a real-valued univariate function or time series (Higuchi, 1988). This Higuchi fractal dimension has since become very popular as a simple fractal dimension estimator allowing the characterization of the scaling behavior of univariate time series. Besides numerous applications across various fields of science, several extensions of the classical framework have been developed during the past years, including a recent generalization to numerically estimating multifractal spectra from time series (Carrizales-Velazquez et al., 2022).

Here, we propose a novel extension of this multifractal Higuchi dimension analysis (MF-HDA) from one-dimensional time-series to two-dimensional image objects. We start by analyzing the properties of a recent two-dimensional generalization of the classical monofractal Higuchi method (Spasic, 2014), revealing some potentially misinterpreted geometric aspects of that original work. A minor modification is proposed to replace the concept of area by a new quantity that has a straightforward connection with the one-dimensional version of the Higuchi fractal dimension and thus provides the basis for a scaling analysis. Subsequently, we present a general mathematical framework for one- and two-dimensional Higuchi fractal dimension estimates and their generalizations to multifractal spectra, following the ideas underlying our previous one-dimensional MF-HDA.

To demonstrate the appropriate behavior of our new two-dimensional MF-HDA, we numerically estimate the multifractal spectra of different paradigmatic examples of mono- as well as multifractal two-dimensional model systems. For the special case of the two-dimensional binomial multifractal cascade model, we show that the results obtained by our new approach are largely consistent with the analytical multifractal spectra. Moreover, we find that our new approach does not exhibit an artificial widening of the multifractal spectra that is observed when applying a two-dimensional multifractal detrended fluctuation analysis as a numerical benchmark algorithm. Finally, we present some selected examples of applications of our approach to different two-dimensional geoscientific and environmental datasets like satellite images, illustrating the potential of systematic applications of our new two-dimensional MF-HDA method.

C. Carrizales-Vazquez, R.V. Donner & L. Guzman-Vargas, Generalization of Higuchi’s fractal dimension for multifractal analysis of time series with limited length, Nonlinear Dynamics, 108, 417-431, 2022.
T. Higuchi, Approach to an irregular time series on the basis of the fractal theory, Physica D, 31, 277-283, 1988.
S. Spasic, On 2D generalization of Higuchi’s fractal dimension, Chaos, Solitons & Fractals, 69, 179-187, 2014.

How to cite: Carrizales-Velazquez, C., Guzmán-Vargas, L., and Donner, R. V.: A new two-dimensional extension of the generalized Higuchi estimator for multifractal data: Theory and application to geoscience problems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14733, https://doi.org/10.5194/egusphere-egu26-14733, 2026.

EGU26-17143 | ECS | Posters on site | NP4.4

SURD-based causal decomposition for nonlinear modeling from multivariate time series 

Kazuki Kohyama, Ryo Araki, Rin Irie, Helen Stewart, and Masaki Hisada

Natural phenomena, such as air–sea interactions, result from complex interactions among many components. Faithfully capturing such interactions is essential for improving predictive and inferential skills. However, identifying variable relationships directly in multivariate time series remains highly challenging. To address this, we specifically prioritize causality, defined as temporal precedence and directed influence, not mere correlation. This is key to identifying mechanisms governing time evolution.

In our previous work, we used transfer entropy (TE) to infer causal structure and reconstruct nonlinear dynamical models exemplified by the Lorenz system from multivariate time series [1]. Through this approach, linear terms were accurately recovered, but multiplicative nonlinear terms proved difficult to reconstruct. We attribute this limitation to the fact that TE primarily quantifies directed information flow between two variables [2], but does not explicitly decompose multi-variable interaction effects (e.g., multiplicative couplings) within the information transfer. This shortcoming motivates the use of a causality framework that can separate redundant, unique, and synergistic contributions, thereby isolating nonlinear interaction effects. Synergistic-Unique-Redundant Decomposition (SURD) decomposes causality into redundant, unique, and synergistic information components in multivariate time series [3]. We use SURD as a causal analysis tool to validate its applicability to data-driven modeling and event-focused observational analysis relevant to tipping or critical transition dynamics.

In this study, we apply SURD-based causal decomposition to time series data generated from low-dimensional nonlinear differential equations. Synergy-dominant driver pairs are used to screen candidate multiplicative terms, which then constrain a sparse model-identification step (e.g., SINDy), improving recovery of nonlinear terms compared with pairwise TE-guided screening alone. While Martínez-Sánchez et al. (2024) primarily established SURD as a causality decomposition framework [3], the present study examines how SURD outputs can be leveraged to support reconstruction of nonlinear model equations, following our previous work, in which we implemented a data-driven approach to identify basis functions to reproduce multivariate time series [1].

We demonstrate this approach on the Lorenz63 and Rössler systems and satellite observation datasets. Concretely, we define the effect variables in the causal analysis as instantaneous tendencies (e.g., dx/d= (x(t+∆t) − x(t))/∆t) rather than one-step-ahead states. We then quantify how candidate drivers contribute to each tendency using an appropriate lag time ∆t corresponding to causal delay. In this setting, synergistic components highlight interaction effects as nonlinear terms that require joint knowledge of multiple drivers. Unique components support single-source linear term contributions, whereas redundant components capture shared explanatory information among drivers. Moreover, we find that applying SURD to time windows extracted immediately before and after tipping yields more discriminative synergy signatures and further improves the reconstruction accuracy of multiplicative nonlinear terms.

Acknowledgments
We thank ALD Lab for the SURD framework (https://github.com/ALD-Lab/SURD) used in this study.

References
[1] K. Kohyama, R. Irie, and M. Hisada, Causal analysis of time series data for modeling nonlinear phenomena, EGU General Assembly 2025, EGU25-3480 (2025).
[2] T. Schreiber, Measuring information transfer, Physical Review Letters, 85(2), 461 (2000).
[3] C. Martínez-Sánchez, G. Arranz, and A. Lozano-Durán, Decomposing causality into its synergistic, unique, and redundant components, Nature Communications, 15(1), 9296 (2024).

How to cite: Kohyama, K., Araki, R., Irie, R., Stewart, H., and Hisada, M.: SURD-based causal decomposition for nonlinear modeling from multivariate time series, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17143, https://doi.org/10.5194/egusphere-egu26-17143, 2026.

Detrended fluctuation analysis (DFA), introduced by Peng et al. in 1994, along with its numerous algorithmic variants and multifractal extensions have become standard tools in nonlinear time series analysis and have found a vast body of applications across a wide range of scientific disciplines. However, many successful applications have in common that the time series under study are of sufficient length and exhibit unique scaling characteristics that are not overprinted by the action of any external dynamical factors. However, the latter two conditions can be violated in the context of complex geoscientific time series. In this work, we are interested in how such situations affect the general behavior of the resulting detrended fluctuation functions and attempt to provide a mechanistic explanation of the observed features, expanding on previous works that have largely been based on the thorough analysis of different kinds of stochastic model systems.

As a paradigmatic example for geoscientific data with particularly complex variability properties, we focus on a time series of satellite altimetry based global mean absolute sea-level variations (GMSL), which is available for the period from 1993 to present day at multi-day temporal resolution. This time series exhibits a variety of non-trivial fluctuation properties, including seasonality and a long-term nonlinear trend, but also reflections of nonlinear inter-annual climate variability modes like the El Nino-Southern Oscillation (ENSO) and Pacific Decadal Oscillation (PDO). While the first two components can be largely removed from the time series by standard approaches like phase averaging and detrending/smoothing, the latter two manifest in GMSL in more subtle manners. We show that the resulting fluctuation functions of GMSL obtained with different orders of local detrending indeed do not exhibit simple and unique scaling characteristics across the full range of accessible scales, even when being subject to de-seasoning and de-trending prior to analysis. Instead, we find that depending on the scale considered, the scale-local fluctuation exponents exhibit a marked pattern, with consistent values across different DFA orders exclusively being observed below multi-annual to sub-decadal time scales. We present a simplistic explanation of those findings by studying the fluctuation functions for different types of stochastic signals with superposed oscillatory components with periodicities resembling those of the different variability modes in GMSL. Additionally, we discuss the potentials and limitations of different statistical approaches (including regression on potential external drivers as well as different time-scale decomposition techniques) to remove the effects of complex externally driven oscillatory modes from the original time series to obtain a more realistic picture of the intrinsic stochastic fluctuation properties of GMSL.

This work was partially supported by INESC TEC via the International Visiting Researcher Programme 2024 and by CMUP - Centro de Matemática da Universidade do Porto, member of LASI, which is financed by national funds through FCT - Fundação para a Ciência e a Tecnologia, I.P., under the project with reference UID/00144/2025. Doi: https://doi.org/10.54499/UID/00144/2025.

How to cite: Donner, R. V. and Matos, J.: Potentials and limitations of detrended fluctuation analysis for complex geoscientific time series: The case of global mean sea-level, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19726, https://doi.org/10.5194/egusphere-egu26-19726, 2026.

Understanding how Arctic climate variability is organized internally and how it connects to large-scale atmospheric variability remains a challenge. Approaches based on indices or dominant modes are well-suited to identifying coherent patterns but offer limited insight into localized connectivity, pathway structure, and the timing of interactions across regions.  Here, we apply a climate network approach to examine the seasonal organization of Arctic atmospheric connectivity using mid-tropospheric circulation (500 hPa geopotential height, Z500) and near-surface air temperature (T2M) over 1940–2024. The analysis focuses on winter (DJF) and summer (JJA), and examines both instantaneous and time-lagged relationships in the free atmosphere and at the surface.  We find a pronounced seasonal dependence in Arctic connectivity. Within the Arctic, Z500 networks exhibit strong and spatially extensive connectivity in winter, consistent with basin-scale coherence in the mid-tropospheric circulation. In summer, this structure weakens and becomes more fragmented. In both seasons, betweenness centrality is broadly distributed, suggesting that Arctic circulation variability is not dominated by a small number of preferred internal pathways. In contrast, T2M networks are more heterogeneous, with spatially uneven connectivity and localized regions of higher importance, highlighting the role of surface conditions in shaping near-surface variability.  When only the strongest links (99th percentile threshold) are considered, direct Arctic large-scale connectivity is weak in both Z500 and T2M. However, time-lagged analysis shows that connectivity can emerge on delayed timescales, particularly in winter, and is more clearly expressed in the circulation field (Z500) than at the surface (T2M). Overall, this study presents a network-based diagnostic perspective on Arctic atmospheric variability, highlighting the seasonal organization and spatial connectivity that complement traditional mode-based analyses. 

 

How to cite: kulkarni, S. and Agarwal, A.: Complex networks as a diagnostic framework for seasonal organization and spatial connectivity in the Arctic atmosphere. , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20175, https://doi.org/10.5194/egusphere-egu26-20175, 2026.

Large scale climate oscillations (COs) are major explanatory drivers modulating climate systems and water resources across the Globe. Understanding the recurring patterns of Global climate oscillations (GCOs) is crucial for developing predictive models of hydro-climatic variables and management of water resources. In this study seven prominent GCOs of 1950-2025 period namely ElNino Southern Oscillations (ENSO), Pacific Decadal Oscillation (PDO), North Atlantic Oscillation (NAO), Indian Ocean Dipole (IOD), Atlantic Multi-decadal Oscillation (AMO) Arctic Oscillation (AO) and Southern Oscillation Index (SOI) are subjected to Recurrence Quantification Analysis (RQA). Diverse set of RQ measures like laminarity determinism, trapping time, entropy and mean diagonal length are quantified for each of the time series considering the complete time spell. The complexity measures are further quantified for pre- and post- Global climate shifts of 1977-78 and 1998-99. Nino 3.4 Index is found to be the most deterministic and stable pattern irrespective of the time spell chosen for the analysis followed by AMO and PDO indices. IOD and AO indices of post-climatic shifts are showing more complex patterns, SOI is most sensitive to climatic shift while remaining indices showed stable patterns in the post-spells of both the climatic shifts. The insights gained from the study are helpful for proceeding with in-depth studies on selection of CO drivers in predictive modeling, multi-variate risk assessment and the synchronization studies of hydro-climatic extremes.

How to cite: Haroon, M. and Sankaran, A.: Complexity evaluation of Global climatic oscillations using Recurrence Quantification Analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22026, https://doi.org/10.5194/egusphere-egu26-22026, 2026.

EGU26-107 | ECS | Orals | HS3.6

Machine Learning Integration Strategies for Process-based Ecohydrological Modeling: Addressing Epistemic Uncertainties of Water Mixing Dynamics in Tree Water 

Hyekyeng Jung, Chris Soulsby, Songjun Wu, Christian Birkel, and Dörthe Tetzlaff

Compared to process-based models (PBMs), higher prediction accuracy of machine learning models (MLMs) has been repeatedly reported in ecohydrological research. This might indicate the higher efficiency of data-driven MLMs for extracting and generalising information from the data, especially when traditional PBMs are often challenged by epistemic uncertainties in process representation. To preserve ‘modelling as a learning tool’, integrating MLMs into PBMs is a promising avenue to leverage MLMs for data assimilation, and PBMs for holistic explainability of processes across the Critical Zone (i.e., the thin crust of the Earth including vegetation).
One example of an ecohydrological process with high epistemic uncertainties is the mixing mechanism of root uptake water from soils by trees. Due to limited process understanding together with high uncertainties of isotope measurements in trees, usually mixing dynamics in tree water storage in ecohydrological models show poor representation.
Here, we use data from a comprehensive monitoring campaign which has been conducted during the growing season of 2020 at a plot site with two willow trees and grass in southeastern Berlin, Germany, including daily or sub-daily in-situ measurements of hydrological characteristics and stable water isotopes in precipitation, soils, vegetation, and neighboring open water bodies. Using the data, a baseline ecohydrological PBM (EcoHydroPlot) was used to simulate water flow and isotope dynamics across the Critical Zone. In addition, MLMs with different strategies for integration were applied: Firstly, as an additional module to the PBM, a post-hoc result-analyzing MLM was trained with the error of the PBM. Secondly, a hybrid model was built that replaces equations for mixing mechanism of root-uptake water in PBM with a data-driven ML algorithm. An eXplainable AI (XAI) tool was applied to help understand uncertainties in the PBM and process representation in MLM.
By comparing these approaches using different criteria of prediction accuracy and interpretability, we identified an optimal strategy for leveraging MLM capabilities within PBM frameworks in addressing the process of tree water mixing with high epistemic uncertainties, potentially extending the concept of ‘modeling as a learning tool’ to MLM-integrated PBMs.

How to cite: Jung, H., Soulsby, C., Wu, S., Birkel, C., and Tetzlaff, D.: Machine Learning Integration Strategies for Process-based Ecohydrological Modeling: Addressing Epistemic Uncertainties of Water Mixing Dynamics in Tree Water, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-107, https://doi.org/10.5194/egusphere-egu26-107, 2026.

EGU26-928 | ECS | Posters on site | HS3.6

Sensitivity of machine-learning crop-type mapping to feature selection and hyper-parameter tuning. 

Mayra Perez, Frédéric Satgé, Jorge Molina, Renaud Hostache, Ramiro Pillco, Elvis Uscamayta, Diego Tola, Lautaro Bustillos, and Celine Duwig

To improve crop yields and economic incomes, farmers consistently adapt their practices to climate and market fluctuations, resulting in highly variable crop field distribution and coverage in space and time. As these dynamics ilustrate, up-to-date crop-type mapping is essential to understand farmers’ needs and supporting them in adopting sustainable practices. With global coverage and frequent temporal observations, remote sensing data are generally integrated in machine learning models to monitor crop-type mapping dynamics. Unlike physical-based models that rely on straightforward use, the implementation of machine-learning approaches depends on deep interaction with users. In this context, the study assesses the output sensitivity of these models to features selection and hyper-parameter calibration, both of wich rely on user consideration. To do so, Sentinel-1 (S1) and Sentinel-2 (S2) features are integrated into five distinct models (RF, SVM, LGB, HGB, XGB), considering different features selection (VIF and SFS) and hyper-parameter calibration set-up. Results show that pre-process modeling VIF feature selection discards features that wrapped SFS feature selection keeps, resulting in less reliable crop-type mapping compared to using SFS. Additionally, hyper-parameter calibration appears to be sensitive to the input feature and its consideration after any the feature selection improved the crop-type mapping. In this context a three-step nested modelling set-up including a first hyper-parameters calibration followed by a wrapped feature selection (SFS) and another hyper-parameter calibration, lead to the most reliable model outputs. Across the considered region, LGB and XGB (SVM) are the most (less) suitable model for crop-type mapping and models reliability improved when integrated S1 and S2 features rather than the consideration of S1 or S2 alone. Finally, crop-type maps are derived across different regions and periods to highlight the benefits of the proposed method to monitor crops’ dynamics in space and time.

How to cite: Perez, M., Satgé, F., Molina, J., Hostache, R., Pillco, R., Uscamayta, E., Tola, D., Bustillos, L., and Duwig, C.: Sensitivity of machine-learning crop-type mapping to feature selection and hyper-parameter tuning., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-928, https://doi.org/10.5194/egusphere-egu26-928, 2026.

Hydrological modelling is essential for water resource management, decision making, extreme events forecasting, and for advancing an integrated understanding of the water cycle. In this context, two main approaches dominate: physics-based (or process-based) models, which simulate hydrological processes such as streamflow using fundamental physics equations, and data-driven models, which use statistical or machine learning techniques to map inputs to outputs. Although Artificial Intelligence (AI) techniques have shown promising results in predictive accuracy, particularly in data-rich basins, their inherently black-box nature raises concerns about whether their internal representations align with real hydrological processes. This is especially critical when models are applied to extreme events, non-stationary conditions, or scenarios beyond the training distribution, where high performance metrics alone may not guarantee reliable or physically meaningful predictions. In this study, we evaluated the performance of a Long Short-Term Memory (LSTM) model for drought modelling modeling and assessed how effectively it could represent real-world hydrological behavior in the Rio Grande do Sul watersheds available in the Catchment Attributes and Meteorology for Large-sample Studies (CAMELS-BR) dataset. The focus on these basins is particularly relevant given the region's hydrological importance, susceptibility to extreme events (e.g., droughts and floods), and distinct characteristics compared to temperate regions, where most legacy models were developed. The model was trained using data from 55 different basins across the state. This multi-basin approach allows the LSTM to learn universal hydrological patterns while maintaining the ability to predict low flow conditions in individual watersheds. The model inputs combined dynamic hydrological variables (e.g., precipitation and evapotranspiration) with static catchment attributes  (e.g., aridity, soil properties, and topography). Accumulated rainfall features were constructed over 3-30 day windows to capture watershed memory effects as a proxy to soil moisture dynamics. In addition, Explainable AI (XAI) techniques together with hydrological signatures (e.g. runoff ratio, baseflow index and elasticity) were applied to assess the physical soundness of the LSTM model in the region. Following this, the internal structure of the LSTM - particularly the cell states - were analyzed and compared with hydrological behavior (e.g., soil water accumulation, groundwater dynamics, rainfall inputs) in both situations where XAI and hydrological signatures highlighted, or did not highlight, physical consistency. The LSTM’s effectiveness in Brazilian watersheds highlighted its potential as a complementary tool for low flow and drought modelling, offering a valuable alternative for water resources management. XAI analyses and hydrological signatures highlighted the physical soundness of the multi-basin model, but also indicated that improvements were needed, as the internal structure did not consistently track physical hydrological behavior in some cases, hindering the extrapolation of the LSTM model to assess drought conditions in different meteorological settings (e.g., climate change scenarios).

How to cite: Canellas, E., Perdigão, R., Brentan, B., and Rodrigues, A.: Beyond Accuracy: Trustworthy LSTM-Based Hydrological Modelling Assessed with XAI and Hydrological Signatures — A Case Study in Rio Grande do Sul, Brazil, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1116, https://doi.org/10.5194/egusphere-egu26-1116, 2026.

EGU26-1275 | ECS | Posters on site | HS3.6

Diffusion-Based Physics-Aware Modeling of Subsurface Soil Moisture 

Vidhi Singh, Abhilash Singh, and Kumar Gaurav

Accurate characterization of soil moisture at subsurface depths is essential for hydrological modeling, agricultural management, and climate risk assessment. However, in-situ subsurface measurements remain sparse and often discontinuous due to logistical and operational constraints, especially in data-limited regions. This creates a pressing need for approaches that can reliably infer deeper soil moisture states from surface observations, which are more readily available from both remote sensing platforms and ground-based sensors. This study proposes a probabilistic, physics-aware denoising diffusion model designed to estimate soil moisture at subsurface depths using only surface moisture measurements. The model integrates smoothness and curvature regularization terms inspired by Fickian diffusion theory as weak physics to guide the learning process, without requiring explicit or site-specific physical parameters, thereby enhancing its practicality and ensuring broader applicability across diverse hydroclimatic conditions. The model is trained and evaluated across 20 global ISMN (International Soil Moisture Network) sites at 10, 20 and 40 cm depths with hourly observations spanning six distinct Köppen–Geiger climate classes and four high-resolution African stations with 10-min data.

Across global stations, the model demonstrated consistently high predictive skill (R² ranging from 0.91 to 0.99) with lower errors in climates characterized by stable seasonal patterns, and comparatively higher uncertainty in regions affected by freeze-thaw dynamics or monsoonal variability. Benchmarking against 17 state-of-the-art algorithms using Dolan–Moré profiles showed strong and reliable performance across depths and metrics. A stochastic robustness analysis with 30 random seeds and varying ensemble sizes indicated that moderate-sized ensembles provide an effective balance between accuracy and stability. Sensitivity experiments with white, autocorrelated, and structured noise revealed that the 20 cm layer is most susceptible to surface-level perturbations, while deeper layer remain comparatively resilient. The model also highlighted a strong performance on higher-resolution datasets, with prediction errors tightly centered around zero and exhibiting very low standard deviation. The generalisation of the proposed diffusion-based model across spatial, temporal, and climatic variability highlights its potential as a lightweight and transferable alternative for hydrological forecasting in data-scarce or operationally constrained environments.

How to cite: Singh, V., Singh, A., and Gaurav, K.: Diffusion-Based Physics-Aware Modeling of Subsurface Soil Moisture, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1275, https://doi.org/10.5194/egusphere-egu26-1275, 2026.

The Yellow River Basin (YRB) is among the most water-scarce, sediment-laden, and anthropogenically impacted river basins worldwide. Rainfall–runoff and runoff–sediment relationships in the YRB have traditionally been investigated using process-based hydrological models, which are computationally demanding and difficult to apply at large spatial scales. Here, a physics-guided LSTM–GNN (Long Short-Term Memory and Graph Neural Network) framework was proposed to simulate coupled water–sediment processes across the YRB. Using sub-basin delineation and upstream–downstream connectivity derived from the physically based Geomorphology-Based Ecohydrological Model (GBEHM), the framework employs LSTM to learn local runoff and sediment generation within individual sub-basins, and GNN to represent topology-constrained routing along the river network. The coupled model generated monthly streamflow and sediment data for 718 sub-basins over the period 1982–2017. Compared with a baseline model that neglects physical river-network topology (total NSEflow=0.78, NSEsediment=0.62; median NSEflow=0.09, NSEsediment=0.13), the proposed framework demonstrated significantly improved predictive performance (total NSEflow=0.89, NSEsediment=0.85; median NSEflow=0.42, NSEsediment=0.32) during the test period (2013–2017), especially at stations in large tributaries and the main stream, with high connectivity and large catchment areas. These results show that the proposed LSTM-GNN framework can effectively serve as a surrogate of the process-based model with high accuracy, highlighting its potential for simulating upstream–downstream coupled hydrological processes in super-large river basins.

How to cite: Li, S., Yang, H., Wang, T., and Yang, D.: Coupled Water–Sediment Modelling in the Yellow River Basin Using a Physics-Guided LSTM–GNN Framework Incorporating River Network Topology, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2784, https://doi.org/10.5194/egusphere-egu26-2784, 2026.

Vegetation mapping is a key step in wetland monitoring, management, and conservation. Remote sensing image classification offers an excellent solution for vegetation mapping due to its high temporal and spatial resolution. In spite of these advantages, remote sensing classification of wetland vegetation is usually limited to a small number of target classes and lack explanation of the input features importance. To address this limitation, this study presents a detailed wetland vegetation classification, which is followed by an explainability study.

The study was conducted in the Biebrza wetlands located in NE Poland, covering approximately 220km2. These wetlands are situated around the Biebrza River, which floods yearly, producing a characteristic vegetation zonation. The training and validation data for vegetation classification was a vegetation survey conducted in 2015 and kindly provided by the Biebrza National Park.

The input features for classification was obtained from fusing VIS-IR data from Sentinel-2, thermal data from Landsat-8, and Synthetic Aperture Radar (SAR) data from Sentinel-1. The Sentinel-2 data consisted of four images (one image per season), each with eleven bands. The Landsat-8 data also comprised four images, with one thermal band per image. The Sentinel-1 data included 24 dual-polarization (VV+VH) images (one image per month, varied by ascending and descending orbit). All image data were acquired within the 2014-2017 period and resampled to 10-meter spatial resolution.

The "ranger" Random Forest implementation in R was used as the classifier. The classifier was trained on a stratified random 50% of the vegetation data points and validated on the remaining 50%. The built-in permutation feature importance algorithm was used to indicate the most important bands for the classification.

The classification-based vegetation map highly reflected the characteristic vegetation zonation of the Biebrza wetlands. The overall accuracy was 0.994 and the Kappa index was 0.993. The most important band for the classification was the Landsat-8 thermal image from the winter season. However, the thermal bands from the remaining seasons were relatively unimportant. The next most important bands were the Sentinel-2 VIS-IR images from the spring and fall seasons, particularly the red, red-edge, and SWIR bands. The SAR data from Sentinel-1 were the least important of all data used; the most important Sentinel-1 band (19th position) was VH from September, descending orbit.

How to cite: Berezowski, T.: Explainable machine learning for detailed wetland vegetation classification using remote sensing data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5240, https://doi.org/10.5194/egusphere-egu26-5240, 2026.

EGU26-5408 | Orals | HS3.6

Global estimation of the median annual maximum flood (QMED) using explainable machine learning  

Valeriya Filipova, David Leedal, and Sam Clayton

Reliable estimation of the median annual maximum flood (QMED) is central to flood risk assessment and the design of hydraulic infrastructure, particularly in ungauged basins. Traditional index-flood approaches typically delineate homogeneous regions and estimate QMED using linear regression on a small set of catchment descriptors. However, these assumptions are often violated in practice, leading to substantial prediction uncertainty. 

Here, we explore the potential of explainable machine-learning models to estimate QMED at large scale. Using data from approximately 8,500 catchments and more than 60 climatic, physiographic, and geomorphological descriptors, we train non-linear models (XGBoost and TabNet) to predict QMED for ungauged basins. To promote physically plausible behaviour, model training incorporates constraints on specific discharge alongside standard performance metrics. A key feature of the approach is the extensive use of DEM-derived terrain and river-network descriptors, which can be computed consistently from widely available global elevation datasets. 

Model interpretability is addressed using global and local explainability techniques, enabling identification of the dominant controls on QMED and how their importance varies spatially. Across independent test data, the models show strong predictive skill (R² > 0.8, median absolute percentage error ~30%). Notably, in many regions models trained on large, globally diverse datasets outperform those trained solely on local data, even where substantial local records are available. 

These results indicate that combining globally consistent physiographic information with interpretable, non-linear machine-learning models offers a promising alternative to traditional regional regression methods for QMED estimation, with potential benefits for flood risk assessment in data-sparse regions. 

How to cite: Filipova, V., Leedal, D., and Clayton, S.: Global estimation of the median annual maximum flood (QMED) using explainable machine learning , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5408, https://doi.org/10.5194/egusphere-egu26-5408, 2026.

EGU26-5540 | ECS | Posters on site | HS3.6

A Deep Ensemble Learning Framework with Interpretability for Long-Term Streamflow Forecasting under Multiple Uncertainties 

Xinyuan Qian, Ping-an Zhong, Bin Wang, Yu Han, Yukun Fan, Yiwen Wang, Sunyu Xu, Zixin Song, and Mengxue Ben

Accurate and reliable long-term streamflow forecasting plays a crucial role in sustainable water resource management and risk mitigation. However, forecast performance is often constrained by multiple sources of uncertainty and the limited interpretability of deep learning models. To address these challenges, this study proposes an explainable hierarchical optimisation framework for long-term streamflow forecasting based on ensemble learning. The proposed framework systematically integrates a Dempster–Shafer (DS) evidence theory-based predictor selection strategy to reduce input uncertainty, an improved loss function designed to enhance model sensitivity to extreme flow events, and a Stacking ensemble scheme that combines the complementary strengths of multiple deep learning models, thereby overcoming the limitations of individual models in complex hydrological systems. In addition, SHapley Additive exPlanations (SHAP) are employed to improve model interpretability and to quantify the contributions of different predictors.

The effectiveness of the proposed framework is demonstrated through long-term streamflow forecasting at Hongze Lake. The results indicate that: (1) the DS-based predictor selection method substantially enhances both forecasting accuracy and stability, with Nash–Sutcliffe efficiency (NSE) values increasing by 0.10–0.18; (2) the improved loss function significantly strengthens model robustness under extreme high-flow conditions, reducing the mean absolute percentage error (MAPE) by 63.11%, 55.33%, and 23.6% for the MLP, LSTM, and Transformer models, respectively; (3) the Stacking ensemble model consistently outperforms individual base models by reducing forecast errors (RMSE decreased by 17–25%), improving the representation of large-scale variability (MAPE reduced by 21.6–26.8%), and more accurately capturing streamflow dynamics (NSE increased by 0.12–0.20), effectively mitigating multi-source uncertainties; and (4) SHAP-based interpretability analysis reveals pronounced monthly variations in predictor importance and confirms the dominant influence of antecedent streamflow on long-term forecasts. Overall, the proposed framework markedly improves the accuracy, robustness, and transparency of long-term streamflow forecasting and shows strong potential for application in other data-driven hydrological forecasting tasks.

How to cite: Qian, X., Zhong, P., Wang, B., Han, Y., Fan, Y., Wang, Y., Xu, S., Song, Z., and Ben, M.: A Deep Ensemble Learning Framework with Interpretability for Long-Term Streamflow Forecasting under Multiple Uncertainties, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5540, https://doi.org/10.5194/egusphere-egu26-5540, 2026.

EGU26-5830 | ECS | Posters on site | HS3.6

Global groundwater recharge estimation through hybrid modeling 

Jiaxin Xie, Zavud Baghirov, Markus Reichstein, and Martin Jung

Groundwater provides drinking water for billions and supports nearly half of irrigated agriculture, yet global renewable groundwater availability—quantified as groundwater recharge—remain highly uncertain. Here, we simulate global groundwater recharge using a hybrid model that seamlessly integrates machine learning with physical processes. The hybrid model substitutes machine learning for poorly represented hydrological processes while retaining established physical equations, such as water balance. By leveraging diverse Earth system observations—including streamflow-derived groundwater discharge, satellite-retrieved terrestrial water storage anomalies, and flux tower evapotranspiration—the hybrid model effectively integrates process knowledge with multi-source data constraints to improve the accuracy of global groundwater recharge simulations. Such integration may also deepen our process understanding of groundwater recharge.

How to cite: Xie, J., Baghirov, Z., Reichstein, M., and Jung, M.: Global groundwater recharge estimation through hybrid modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5830, https://doi.org/10.5194/egusphere-egu26-5830, 2026.

Soil moisture is a fundamental hydrological variable that governs groundwater recharge and agricultural productivity. Accurate long-term forecasting is essential for water resource management, yet it remains challenging due to significant observational noise in sensor data and the error propagation inherent in traditional deep learning models. While physics-based models struggle with site-specific calibration and Neural Ordinary Differential Equations (Neural ODEs) often fail to recover stable continuous dynamics from noisy, discretely sampled signals, there is a clear need for a more robust forecasting framework.

In this work, we propose EulerNet, a pragmatic discrete-time framework designed for high-fidelity soil moisture prediction. Instead of attempting to reconstruct complex latent continuous-time vector fields, EulerNet explicitly models the fixed-step mapping required for operational forecasting. The architecture integrates an Euler-style residual update to parameterize one-step tendencies, ensuring numerical stability through its incremental integration form. To mitigate the impact of sensor noise, we incorporate a Random Synthesizer feature mixer. By employing input-independent alignment matrices rather than dynamic self-attention, the Random Synthesizer acts as an implicit regularizer, preventing the model from overfitting to spurious, noise-induced correlations.

We evaluated EulerNet using high-noise in-situ observations. In a one-month autoregressive rollout, the model achieved exceptional performance with R2 = 0.7977, RMSE = 0.0039, and RMAE = 0.0083. These results demonstrate that for fixed-step environmental forecasting, a specialized discrete-time formulation can effectively bypass the complexities of continuous-time modeling while maintaining high stability and accuracy under significant noise. Our findings provide a practical and efficient alternative for modeling complex Earth system dynamics from real-world observational data.

How to cite: Kang, W.: EulerNet: A Robust Discrete-Time Framework for Long-Term Soil Moisture Forecasting Under Significant Observational Noise , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8707, https://doi.org/10.5194/egusphere-egu26-8707, 2026.

Accurate rainfall-runoff analysis is vital for flood prediction, water resources management, and climate impact assessment. While data-driven hydrological models such as Long Short-Term Memory (LSTM) networks have shown promise, developing a globally applicable framework that is accurate, interpretable, and computationally efficient remains a grand challenge, primarily because most catchments worldwide are ungauged. We address this by employing HYdrologic Prediction with multi-model Ensemble and Reservoir computing (HYPER). This hybrid method combines Bayesian Model Averaging (BMA), a multi-model ensemble, with Reservoir Computing (RC), a type of machine learning model. The framework infers model weights for ungauged basins by linking catchment attributes to the model weights learned from gauged basins. While this model has previously demonstrated higher accuracy and lower uncertainty compared to LSTMs, particularly when training data is limited, its global applicability remains unassessed. Therefore, in this study, we evaluate the global applicability of HYPER using a pseudo-ungauged approach, where gauged basins are treated as ungauged for validation. We challenge the conventional assumption that more data is better by investigating whether selecting a strategic subset of gauged basins for training outperforms using the entire available dataset. Initial experiments revealed that prediction accuracy remained robust regardless of whether 90 % or only 3 % of available basins were used for training. Furthermore, training on basins from a single, hydrologically similar region often yielded higher accuracy than training on a diverse multi-regional dataset. To identify the optimal training subset, we compared three distinct data selection methods: 1) Greedy selection, which identifies donor basins by selecting the nearest neighbors within the static catchment attribute state space; 2)  Physics-Informed selection, which calculates the distance between target and candidate basins while applying heavier penalty weights to slope and aridity to strictly enforce physical similarity; and 3) Meta-Learning, which utilizes a Random Forest to learn the relationship between attribute differences and model weight correlations, subsequently predicting donor basins expected to have the highest weight correlation with the target. While all three methods outperformed the baseline of using all available data (Kling-Gupta Efficiency (KGE): 0.12), the Physics-Informed and Meta-Learning approaches achieved the highest consistency and accuracy. Even when only 5 out of 1,505 basins were used for training, these methods achieved KGE scores of 0.26 and 0.31, respectively, effectively bridging the performance gap toward fully gauged basins (KGE: 0.54). These findings demonstrate that for global prediction in ungauged regions, data quality, especially the strategic selection of training basins, is more important than data quantity, marking a step towards robust, globally applicable runoff analysis.

How to cite: Funato, M. and Sawada, Y.: Data Quality over Quantity: Optimized Data Selection for Data-driven Global Prediction in Ungauged Basins, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9189, https://doi.org/10.5194/egusphere-egu26-9189, 2026.

EGU26-10856 | ECS | Orals | HS3.6

Calibration of a Long Short-Term Memory (LSTM) rainfall-runoff model using remote sensing soil water content estimations 

Tibor Rapai, Petra Baják, István Gábor Hatvani, András Lukács, and Balázs Székely

Long Short-Term Memory (LSTM) neural networks have proven their excellence in basin-level discharge prediction, provided there is an adequate amount of high-quality time series data available for training, including meteorological forcings and streamflow gauge measurements. Such data-driven black-box models can successfully learn the complex behavior of delayed hydraulic responses; however, they cannot yet be easily applied in water management practice, and model transfer attempts to ungauged catchments have not been entirely successful.

In our previous work, we explored an approach to characterizing near-surface flow regimes, starting from a full catchment model and then applying a single LSTM network layer within a semi-distributed subbasin setup reflecting downstream topography. Application to the Tarna River catchment area in Hungary (2,116 km2) showed that transfer learning from the full catchment model (achieving an NSE of 0.91 on the training set and 0.66 on an independent test set) to a downstream chain of gauged Hydrological Response Units (HRUs) is a powerful tool for investigating a semi-distributed HRU network. The entire setup, however, involves a much higher level of complexity, and the available detailed meteorological data and gauge measurements in only two-thirds of the subbasins did not provide sufficient information for the single LSTM model to fully predict the HRU network processes.

Because these models apply “virtual water amounts” stored in the hidden cells of the LSTM network for discharge estimation, their internal variables lack direct physical interpretability. In the present research, we investigate how data fusion during calibration with Gravity Recovery and Climate Experiment (GRACE) data, downscaled using soil water content and evapotranspiration products from the ECMWF Reanalysis (ERA5) database, can improve predictive performance, and help to verify our working hypothesis regarding the theoretical connection between Near Surface Water Content (NSWC) and LSTM cell states.

These results can also validate interpretations derived from our model concerning baseflow contributions and recharge-discharge classification of subbasins, while promising realistic transferability of the pre-trained lumped catchment model to all subbasins and broader general applicability of the proposed method. We hypothesize that the daily change dynamics of Terrestrial Water Storage (TWS) and NSWC – the latter playing a decisive role in gravitational flows within the Critical Zone – are strongly correlated.

Accordingly, we propose using downscaled TSW estimates to (1) introduce a new term into the loss function based on our working hypothesis relating median LSTM cell state values to the normalized dynamics of NSWC, and (2) add a new input dimension approximating total runoff as precipitation minus evapotranspiration and infiltration.

Furthermore, the current model extension, still based on 0.1 ° gridded input data, prepares the ground for future developments that incorporate high-spatial-resolution satellite remote sensing data, such as Sentinel-2 NDWI, to support local-scale hydrological applications efficiently. Integrating satellite data products with different temporal and spatial resolutions is not a straightforward calibration step for rainfall-runoff models, as pixel-wise normalization of measurements requires complex physically based geostatistical methods compatible with model logic to avoid performance deterioration.

 

How to cite: Rapai, T., Baják, P., Hatvani, I. G., Lukács, A., and Székely, B.: Calibration of a Long Short-Term Memory (LSTM) rainfall-runoff model using remote sensing soil water content estimations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10856, https://doi.org/10.5194/egusphere-egu26-10856, 2026.

EGU26-12259 | ECS | Posters on site | HS3.6

Global Rooting Depth Inferred based on Machine Learning 

Shekoofeh Haghdoost, Shujie Cheng, Oscar Baez-Villanueva, and Diego G. Miralles

Rooting depth Zr is a key variable controlling plant water uptake, soil–vegetation interactions, and land–atmosphere feedbacks. Despite its importance, global estimation of Zr remains challenging due to sparse in situ observations and strong spatial heterogeneity driven by climatic, edaphic, and vegetation controls. The interaction among these factors increases complexity, limiting the performance of traditional process-based models and leading to substantial uncertainty in large-scale applications. In this context, machine learning offers a data-driven alternative that can integrate heterogeneous datasets and capture nonlinear relationships and complex interactions among environmental variables, providing a flexible framework for improving large-scale estimates of rooting depth.

In this research, we investigate the environmental drivers of rooting depth at the global scale and develop a new spatially explicit Zr dataset using advanced machine learning methods. Our framework integrates multiple globally consistent datasets, including satellite-derived vegetation metrics (LAI, NDVI), land-surface temperature, and gridded climate variables (precipitation, radiation). These are complemented by soil hydraulic and physical attributes from global soil databases and detailed topographic information, providing a complete representation of environmental controls relevant to rooting depth. A Random Forest model is employed to capture the nonlinear relationships between the predictor set and observed rooting depths. Model interpretability is subsequently assessed using Shapley Additive exPlanations (SHAP), thereby quantifying the contribution of each environmental variable to model predictions.

The optimized model is subsequently applied at the global scale to generate a global Zr dataset using globally available plant, soil, and climate variables. By accounting for their combined effects, the model provides a spatially continuous representation of rooting depth across diverse regions. Model performance is evaluated using leave-one-out cross-validation (LOOCV), whereby each observation is iteratively excluded from the training dataset and used for independent validation. In addition, the resulting predictions are compared against existing global rooting depth datasets to evaluate large-scale consistency. The new Zr dataset enables improved drought monitoring capabilities through more realistic estimates of plant available water; it may enhance water resource assessments by refining infiltration and groundwater recharge estimates, and it helps reduce uncertainty in land surface and climate models by better representing soil-vegetation interactions. Overall, this work provides a robust data-driven approach for estimating Zr globally, independent of process-based assumptions, and relevant for diverse ecohydrological applications striving towards more accurate characterizations of terrestrial water and carbon cycling.

Keywords: rooting depth, machine learning, soil vegetation interactions, global hydrology, ecohydrology, Earth system modeling

How to cite: Haghdoost, S., Cheng, S., Baez-Villanueva, O., and G. Miralles, D.: Global Rooting Depth Inferred based on Machine Learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12259, https://doi.org/10.5194/egusphere-egu26-12259, 2026.

EGU26-12581 | ECS | Posters on site | HS3.6 | Highlight

Causal Analysis for Model Evaluation in Large Sample Hydrology 

David Strahl, Urmi Ninad, Sebastian Gnann, Karoline Wiesner, and Thorsten Wagener

Hydrological and land surface models rely on strong prior assumptions about system functioning, including which processes are represented, their parametrization and how they are simplified across space and time. Model evaluation, however, is often based on measures of predictive performance that provide limited insights into whether models capture underlying processes correctly. Causal discovery methods offer a complementary perspective by learning causal interaction networks directly from time series data to reveal how system components influence each other. Here, we apply the PCMCI+ algorithm for causal discovery in combination with a causal effect estimation to hydrometeorological observations and model simulations from 671 U.S. catchments to infer monthly causal interaction networks and associated effect strengths. We show that inferred interaction strengths vary systematically across gradients of water and energy availability and reflect structural differences in how three hydrological models represent key processes of snow and evapotranspiration dynamics. Our results illustrate how causal inference can complement traditional model evaluation approaches in complex environmental systems by providing process-level insights that help bridge theory, observations, and models across disciplines.

How to cite: Strahl, D., Ninad, U., Gnann, S., Wiesner, K., and Wagener, T.: Causal Analysis for Model Evaluation in Large Sample Hydrology, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12581, https://doi.org/10.5194/egusphere-egu26-12581, 2026.

EGU26-17878 | Posters on site | HS3.6

Estimating the timing of the peak snowmelt floods in unregulated boreal catchments using machine learning techniques. 

Sadegh Kaboli, Ville Kankare, Cintia Bertacchi Uvo, Petteri Alho, Ali Torabi Haghighi, and Elina Kasvi

The timing of peak snowmelt floods in boreal environments has undergone significant changes, characterized by nonlinear and complex patterns. This timing determines when coastal areas of boreal rivers experience the greatest inundation during the spring season. It is highly sensitive to climate change and directly influences local fauna and flora. Despite its critical role in flood risk management, the prediction of spring flood timing, along with the identification of its key drivers and most influential factors, remains insufficiently studied in boreal regions.

In this study, we investigate the potential for predicting the timing of annual maximum snowmelt floods by applying a thermal definition of the spring season, along with various climatological and hydrological indices. The analysis is based on a comprehensive daily dataset available with varying record lengths of at least 50 years, available since the early 1960s and extending to 2023 across multiple unregulated Finnish catchments. Among the most important dynamic features are daily discharge records, high-resolution gridded temperature data, and atmospheric teleconnection indices. Additionally, key static catchment characteristics, such as area, slope, and geographical position, are also incorporated into the modeling process, along with other relevant variables.

Machine learning algorithms, including Random Forest and SHAP (SHapley Additive exPlanations) values for feature importance, are applied to identify the most influential factors shaping the timing of annual maximum snowmelt floods and to assess the overall predictability of these events across multiple catchments. The study introduces a novel approach using a thermal definition of spring. The findings provide new indices and actionable thresholds that can help identify areas where adaptation measures should be prioritized.

How to cite: Kaboli, S., Kankare, V., Bertacchi Uvo, C., Alho, P., Torabi Haghighi, A., and Kasvi, E.: Estimating the timing of the peak snowmelt floods in unregulated boreal catchments using machine learning techniques., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17878, https://doi.org/10.5194/egusphere-egu26-17878, 2026.

EGU26-17916 | ECS | Orals | HS3.6

Combining LSTMs with a Single-Model Large Ensemble for Runoff and Water Temperature Projections in Bavaria 

Alexander Sasse, Ralf Ludwig, Julius Weiß, and Kerstin Schütz

Both river runoff and river water temperature are experiencing highly dynamic alterations, posing serious threat to aquatic ecosystems and water resources management under climate change. Data-driven models such as Long Short-Term Memory (LSTM) networks have demonstrated remarkable skill in hydrological prediction, yet their application under non-stationary climate conditions remains challenging due to limited generalization to unseen catchments and conditions beyond the training distribution. We address these challenges by combining LSTM architectures with single-model initial condition large ensemble (SMILE) climate projections to assess non-stationary, non-linear hydrological responses considering the full range of internal climate variability and climate change, enabling robust assessment of rare and extreme events in Bavaria, Germany.

Our study builds on the ClimEx project, which provides a 50-member ensemble of climate simulations (1950–2099, RCP8.5 emission scenario) at 12 km resolution over Europe using the Canadian Regional Climate Model CRCM5.

We present two complementary application cases operating daily and at 3-hourly temporal resolution: i) For discharge prediction, we train an LSTM on observed runoff across 98 Bavarian catchments, validated against simulations from the process-based Water balance Simulation Model (WaSiM). The architecture processes dynamic meteorological forcings through stacked LSTM layers while incorporating static catchment attributes, using a composite loss function that balances performance across high and low flows. The trained model is then driven by the ClimEx ensemble to generate probabilistic discharge projections for future climate. ii) For water temperature (Tw) prediction, we developed an Entity-Aware LSTM (EA-LSTM) framework trained on observations from 44 Bavarian gauging stations, a subset of the 98 catchments constrained by Tw data availability, extended with nine French river basins to broaden the climatic gradient encountered during training. The EA-LSTM architecture explicitly separates static catchment attributes (elevation, slope, upstream river length) from dynamic meteorological forcings, using static features to parameterize the input gate rather than concatenating them at every timestep. This allows the network to learn site-specific temporal dynamics without overfitting individual locations.

To enhance model interpretability, we apply explainable AI (XAI) techniques including permutation-based feature importance analysis. Results reveal that air temperature and radiation dominate Tw predictions overall, while topographic attributes gain importance under thermal extremes, indicating the model captures physically meaningful process controls. Additionally, robustness tests with perturbed static inputs confirm smooth performance degradation rather than abrupt collapse, suggesting the EA-LSTM learns generalizable attribute-response relationships rather than memorizing site identities.

Both cases demonstrate how combining diverse training data with ensemble-based climate projections enables more robust predictions of hydrological extremes under climate change, while XAI methods provide transparency into learned representations.

How to cite: Sasse, A., Ludwig, R., Weiß, J., and Schütz, K.: Combining LSTMs with a Single-Model Large Ensemble for Runoff and Water Temperature Projections in Bavaria, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17916, https://doi.org/10.5194/egusphere-egu26-17916, 2026.

EGU26-18384 | Orals | HS3.6

Physics-constrained or physics-ignored? An entropy-based approach to diagnose if your hybrid model effectively skips conceptual constraints 

Anneli Guthke, Manuel Álvarez Chaves, Eduardo Acuna Espinoza, and Uwe Ehret

Despite great success of deep learning models in many applications of hydrological prediction, they still face limitations in predicting extreme events or in generalizing to unseen conditions, which raises questions about their fidelity and applicability beyond purely operational purposes. Physics-informed hybrid modelling is often proposed as a way to install interpretability and enable trustworthy data-driven predictions that are in agreement with theoretical knowledge. Yet, the community is still in search of best practices for how to construct physics-informed machine learning models – several “entry points” for physics knowledge exist, i.e., the loss function, the model inputs, or the architecture. Here, we focus on the latter, and on arguably the most “constrained” form of bringing in physics into a hybrid model: a traditional, process-based (conceptual) hydrological model is combined with a data-driven component (here: a long short-term memory network, LSTM) that modifies its parameters over time, as learned by training on observed discharge values. For this apparently well-constrained scenario of hybrid modelling, we raise the question if it can faithfully be called “physics-constrained”, or if the data-driven component is able to overwrite these constraints for the sake of increased performance.

To objectively address this question, we introduce an entropy-based method to quantify the “activity” of the data-driven component in acting against the conceptual constraints. This metric is complemented with a diagnostic workflow to better understand the internal functioning of the resulting, effective hybrid model structure in predicting discharge. Through didactic examples, inspired by real-world case studies, we present the method and build an intuition of what our entropy-based metric represents. Further, we discuss selected results from a large-sample case study on CAMELS-GB to illustrate the variety of findings and insights we had: (1) Performance heavily relies on the data-driven component, and the physics constraints often even make the prediction problem harder instead of adding helpful information; (2) the data-driven component tends to overwrite the constrained architecture “silently”, but this can be detected with our proposed workflow; (3) even nonsensical-at-first-sight constraints can in fact increase performance, as the hybrid model is transformed into a  new structure that is parsimonious and efficient; (4) claiming interpretability on the basis of prescribed constraints is risky at best – before calling a hybrid model of this type interpretable, we should carefully check what’s happening inside. Overall, these findings provide fundamental guidance towards (hybrid) model building and will help us find better ways to reconcile knowledge and information in data for trustworthy models.

How to cite: Guthke, A., Álvarez Chaves, M., Acuna Espinoza, E., and Ehret, U.: Physics-constrained or physics-ignored? An entropy-based approach to diagnose if your hybrid model effectively skips conceptual constraints, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18384, https://doi.org/10.5194/egusphere-egu26-18384, 2026.

Understanding how rainfall is transformed into streamflow is a cornerstone of hydrological science. Despite decades of progress, it remains uncertain whether physical or semi-empirical process equations formulated at the field scale can be transferred to the catchment scale without loss of realism. We assumed that this scale-mismatch is a key reason why conventional conceptual/process-based models often fail to achieve simulation accuracy comparable to purely data-driven deep learning models. Motivated by ensemble rainfall–runoff analysis (ERRA), which suggests that streamflow can be expressed as a convolution between precipitation and a nonlinear catchment response function, we develop an LSTM-based framework to learn catchment-scale response functions for each hydrological process directly from data while retaining physically consistent structure.

The proposed framework couples a generic bucket model architecture with an LSTM that acts as a nexus optimizer. Physical consistency is enforced through residual-style loss regulation, embedding mass-conservation constraints within the training objective. Within this setting, key processes, including canopy interception, infiltration, evapotranspiration, river routing, and groundwater recharge, emerge as extractable functions of meteorological forcing sequences rather than being prescribed a priori. We founded that the learned catchment-scale response functions exhibit pronounced nonlinearity and memory effects. Our results further indicate that catchment-scale process representations effectively mix field-scale empirical relationships with precipitation spatiotemporal heterogeneity, and that the deformation from field to catchment scale response function is strongly driven by the spatial heterogeneity of precipitation intensity. By restructuring the learning pathway to reduce recurrent dependencies, the framework supports efficient parallel training while maintaining physical consistency. The approach aims to simultaneously simulate streamflow and induce catchment scale response functions, offering a pathway to diagnose why conventional models fail and to advance process discovery via data-driven induction.

How to cite: Liu, C.-Y. and Hsu, S.-Y.: Deep Learning as a Nexus Optimizer: Extracting Hydrological Response functions for Rainfall-Runoff Simulation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21276, https://doi.org/10.5194/egusphere-egu26-21276, 2026.

EGU26-4 | ECS | Posters on site | HS6.5

Advanced phycocyanin detection in a South American lake using Landsat imagery and remote sensing 

Lien Rodríguez-López, David Bustos Usta, Lisandra Bravo Alvarez, Iongel Duran Llacer, Luc Bourrel, Frederic Frappart, and Roberto Urrutia

In this study, multispectral images were used to detect toxic blooms in Villarrica Lake in Chile, using a time series of water quality data from 1989 to 2024, based on the extraction of spectral information from Landsat 8 and 9 satellite imagery. To explore the predictive capacity of these variables, we constructed 255 multiple linear regression models using different combinations of spectral bands and indices as independent variables, with phycocyanin concentration as the dependent variable. The most effective model, selected through a stepwise regression procedure, incorporated seven statistically significant predictors (p < 0.05) and took the following form: FCA = N/G + NDVI + B + GNDVI + EVI + SABI + CCI. This model achieved a strong fit to the validation data, with an R2 of 0.85 and an RMSE of 0.10 μg/L, indicating high explanatory power and relatively low error in phycocyanin estimation. When applied to the complete weekly time series of satellite observations, the model successfully captured both seasonal dynamics and interannual variability in phycocyanin concentrations (R2 = 0.92; RMSE = 0.05 μg/L). These results demonstrate the robustness and practical utility for long-term monitoring of harmful algal blooms in Lake Villarrica.

How to cite: Rodríguez-López, L., Bustos Usta, D., Bravo Alvarez, L., Duran Llacer, I., Bourrel, L., Frappart, F., and Urrutia, R.: Advanced phycocyanin detection in a South American lake using Landsat imagery and remote sensing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4, https://doi.org/10.5194/egusphere-egu26-4, 2026.

EGU26-125 | ECS | Orals | HS6.5

Flood Dynamics and Frequency Mapping in the Lower Ganges Floodplain in India Using Multi-Temporal Sentinel-1 SAR Observations (2016–2024) 

Mohammad Sajid, Haris Hasan Khan, Arina Khan, and Abdul Ahad Ansari

The Ganges floodplains are among the most flood-prone regions in India, where recurrent inundations cause significant socio-economic and ecological impacts. Understanding the spatial distribution, frequency, and dynamics of flooding is essential for effective floodplain management and enhancing climate resilience. This study examines the flood frequency and spatial extent across a section of the Ganga River floodplains in Bihar, utilising multi-temporal Sentinel-1 Synthetic Aperture Radar (SAR) data spanning the period from 2016 to 2024. Flooded areas were delineated through an optimal threshold-based classification of VH-polarised backscatter images, with threshold values ranging from -19.5 dB to -22.3 dB. Annual flood extents were mapped, and an inundation frequency composite was generated to identify zones experiencing recurrent flooding. The spatial analysis revealed substantial variability in flood occurrence, with extensive inundation observed in low-lying regions. Several areas were inundated in more than 60% of the study years, indicating chronic flood exposure. The decadal analysis revealed that August and September were the peak months for flooding, with some areas remaining inundated for more than one month, which had an adverse impact on both human settlements and agricultural lands. Validation using optical satellite imagery from Sentinel-2 confirmed a 98% accuracy in the SAR-derived flood extent, reinforcing the reliability of the classification method. The temporal flood frequency analysis provides crucial insights into long-term flood dynamics and helps identify hydrologically sensitive zones. Overall, this study highlights the effectiveness of SAR-based monitoring in understanding floodplain behaviour under changing climatic and hydrological conditions, and supports improved flood hazard mapping, hydrodynamic model calibration, and sustainable flood risk management in the Ganges Basin and other monsoon-affected regions.

Keywords: Flood Inundation, Multi-Temporal, Time-Series, Flood Frequency, Sentinel-1 SAR, Ganges River

How to cite: Sajid, M., Hasan Khan, H., Khan, A., and Ansari, A. A.: Flood Dynamics and Frequency Mapping in the Lower Ganges Floodplain in India Using Multi-Temporal Sentinel-1 SAR Observations (2016–2024), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-125, https://doi.org/10.5194/egusphere-egu26-125, 2026.

Wetlands are very sensitive hydrological ecosystems that are essential for groundwater recharge, flood control, and biodiversity. Climate variability, changed river regimes, and unsustainable anthropogenic pressures are all posing new challenges to their stability. The current work evaluates the two-decade hydro-climatic dynamics of the Haiderpur Wetland (Ganga River, India) by merging optical (Landsat), radar (Sentinel-1), and gridded climate (ERA5, CHIRPS) datasets with GRACE-based groundwater anomalies. On the Google Earth Engine (GEE), processing of time-series Landsat (NDVI, NDWI, LST) and Sentinel-1 (SAR) data to monitor all-weather surface inundation and vegetation structure. To disentangle climatic and anthropogenic drivers, these remote sensing products are statistically correlated against ERA5-Land (Evapotranspiration) and CHIRPS (Precipitation) data, alongside GRACE groundwater anomalies. The findings demonstrated a considerable downward trend in pre-monsoon NDWI and wetland water distribution. This was accompanied by a significant increase in LST and an unexpected increase in NDVI. All-weather Sentinel-1 data validated the drying trend. On the other hand, 'greening' (as indicated by NDVI) in a drying environment suggests a structural shift from native wetland vegetation to more drought-tolerant or invasive terrestrial plants. The study assesses the capability of a multifaceted (optical-radar-climate) GEE strategy to quantify the individual contributions of climatic and anthropogenic factors, while also monitoring wetland development. Furthermore, these findings quantify the hydro-ecological vulnerability of major Ramsar wetlands and emphasize the vital need for coordinated water management to sustain ecosystems in the Ganga River Basin, with far-reaching implications for global wetland conservation.

Keywords: Hydrology, GRACE, Climate Change, SAR, NDVI, NDWI, LST

How to cite: Ansari, A. A., Hasan Khan, H., Khan, A., and Sajid, M.: Hydro-Ecological Vulnerability of  Ganga River Wetland (India): A Multi-Sensor Remote Sensing and GRACE-based Assessment of the Haiderpur Ramsar Site, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-147, https://doi.org/10.5194/egusphere-egu26-147, 2026.

Floods are the costliest and most frequently occurring natural disasters. One of the key factors in preventing and reducing losses is providing a reliable flood map. However, the uncertainty associated with either flood inundation model or data, specifically the Digital Elevation Model (DEM), may have adverse effects on the reliability of flood stage and inundation maps. Therefore, a systematic understanding of the uncertainty is necessary. In this study, an attempt is made to assess whether models are more susceptible to the uncertainties or the data itself. In order to do this, a SCIFRIM (Slope-corrected, Calibration-free, Iterative Flood Routing and Inundation Model) is employed, utilizing a list of DEM datasets to reconstruct the October 2024 Valencia flood event. The modelled flood extents were validated against those derived from multi-sensor remote sensing data. The Critical Success Index (CSI) was calculated to assess the agreement between observed and modelled flood extents, yielding values of 0.49 and 0.59 for October 30th and 31st, respectively, when combining SCIFRIM and Lidar-DEM. Additionally, a multi-model comparison has been performed between SCIFRIM and CaMa-Flood (Catchment-based Macro-scale Floodplain), HEC-RAS (Hydrologic Engineering Center's River Analysis System), and TUFLOW (Two-dimensional Unsteady FLOW), demonstrating its relevance in terms of outputs (flood extent and stage) and model runtime. The findings demonstrate that the proposed modeling framework offers a reliable approach for flood assessment. It has great potential to support rapid assessment and decision-making in data-scarce regions.

How to cite: Tripathi, G., Sarkar, E., and Biswal, B.: Evaluating Slope-corrected, Calibration-free, Iterative Flood Routing and Inundation Model (SCIFRIM)-based Flood Inundation against multi-satellite observation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-436, https://doi.org/10.5194/egusphere-egu26-436, 2026.

Floods are highly dynamic hazards whose spatial extent can change rapidly within hours. Timely and accurate monitoring is essential for early warning, emergency response, and post-disaster assessment. A major challenge in current Earth Observation (EO) based approaches is the difficulty of capturing the complete evolution of a flood event, including its maximum flood extent. This information is often missing due to temporal gaps in Synthetic Aperture Radar (SAR) acquisitions and cloud cover in optical imagery. Missing the peak extent limits the accuracy of impact assessments and poses challenges for applications such as parametric insurance, which depend on reliable measurements of flood magnitude. Although daily flood products exist, they are often based on large-scale multi-spectral sensors and struggle during persistent cloud cover as well as with resolution for smaller events, creating an urgent need for a more reliable method for daily flood estimation from higher-resolution SAR datasets. To address these challenges, we propose a novel deep learning framework that fuses EO-based coarse dynamic hydrometeorological data with static geospatial datasets to produce high-resolution daily flood extent maps. Our approach integrates static flood conditioning inputs, including elevation, Height Above Nearest Drainage, Urban Development Area, flow direction, Normalized Difference Vegetation Index, Normalized Difference Built-up Index, soil clay and sand content, and pre-flood SAR and multispectral imagery with dynamic hydrometeorological variables such as daily precipitation and soil moisture. The model adopts a multi-stage vision transformer architecture: encoders extract multi-level latent representations from all inputs, which are then fused using cosine similarity, normalization, and temporal attention mechanisms. A decoder reconstructs high-resolution flood extent, followed by a Gaussian filter to reduce high-frequency noise. The framework is fully supervised using the globally available KuroSiwo flood mask dataset, ensuring transferability across diverse geographic regions and climate zones. In addition, this research provides a complete data preparation workflow that converts flood mask shapefiles into standardized image patch datasets, including a modular input selection interface that removes dependence on inputs included in specific datasets, directly suitable for deep learning training, enabling straightforward implementation and practical applicability. The model is trained and evaluated across three distinct climate zones on multiple continents, demonstrating a robust capability to overcome the temporal limitations of SAR data and cloud-induced gaps in optical observations. Held-out region tests with strict geographic separation to minimize spatial autocorrelation induced data leakage, further ensure unbiased evaluation and true transferability. Preliminary tests across multiple continents yield stable performance, with cross-site metric variations remaining within approximately 5-7 percent. This study introduces the first deep learning framework for daily fine-scale flood extent mapping using purely EO data which are globally accessible, providing a scalable and transferable solution for real-time flood monitoring, disaster management, and potential applications in parametric insurance by improving flood mapping cadence and reliably estimating maximum flood extents.

Keywords: spatio-temporal fusion, vision transformer, high-resolution flood mapping

How to cite: Surojaya, A., Kumar, R., and Dasgupta, A.: DeepFuse2.0: Novel Deep Learning-based Fusion of Satellite-based Hydroclimatic Data and Flood Conditioning Factors for Daily Flood Extent Mapping, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1047, https://doi.org/10.5194/egusphere-egu26-1047, 2026.

EGU26-1092 | ECS | Posters on site | HS6.5

Cross-Biome Transferability of SAR-based Flood Mapping with Random Forests 

Paul Christian Hosch and Antara Dasgupta

Fully automated, globally applicable flood-mapping systems must earn user trust, which in turn requires systematic testing across diverse environmental conditions to understand performance stability and a clear understanding of model transferability. While some recent studies have evaluated cross-site performance of flood mapping algorithms, the cross-biome transferability of Random Forest (RF) models for SAR-based flood delineation has not yet been thoroughly evaluated. In this study, we assess how well RF classifiers trained for binary flood detection generalize across biomes using primarily Synthetic Aperture Radar (SAR) data. Our feature stack comprises 14 variables, including 9 SAR-derived features (Sentinel-1 VV and VH backscatter and associated temporal-change metrics) which provide information on the flood-induced land surface changes and 4 contextual predictors such as land cover and topographic indices which influence radar backscatter and help to reduce as well as mitigate uncertainties. Experiments were conducted across 18 flood events distributed equally amongst 6 distinct biomes: (1) Deserts and Xeric Shrublands, (2) Tropical and Subtropical Moist Broadleaf Forests, (3) Temperate Broadleaf and Mixed Forests, (4) Temperate Coniferous Forests, (5) Mediterranean Forests, Woodlands and Scrub, (6) Temperate Grasslands, Savannas and Shrublands. Model transferability is evaluated using a two-level nested cross-validation approach. First, intra-biome performance is established through an inner 3-fold Leave-One-Group-Out Cross-Validation (LOGO-CV), in which models are trained on all but one site within a biome and evaluated on the held-out site iteratively. Second, inter-biome transferability is quantified using an outer 6-fold LOGO-CV, treating each biome as a distinct group. In this setup, models are trained on all biomes except one and evaluated on all sites of the held-out biome. Classification performance is assessed using Overall Accuracy (OA), F1-score, Precision, Recall, and Intersection over Union (IoU), with all experiments repeated across 10 independent iterations to capture model structural and sampling variability.

Preliminary results on select biomes show substantial variation in inter-biome transferability. Notably, in some cases, models transferred between biomes outperform those trained within the same biome. These findings highlight the need for comprehensive biome-level transferability assessments to better understand the capabilities and limitations of RF-based flood mapping under globally diverse conditions, ultimately supporting more transparent and trustworthy flood-mapping products for end users.

How to cite: Hosch, P. C. and Dasgupta, A.: Cross-Biome Transferability of SAR-based Flood Mapping with Random Forests, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1092, https://doi.org/10.5194/egusphere-egu26-1092, 2026.

EGU26-1266 | ECS | Posters on site | HS6.5

Cross-Biome Feature Importance Stability Analysis for SAR-based Flood Mapping with Random Forests 

Parisa Havakhor, Paul Hosch, and Antara Dasgupta

Flood mapping using machine learning methods such as Random Forests (RF) requires informed feature engineering and selection. Despite feature-importance rankings across different biomes and land covers varying substantially, the stability of these feature rankings has not been evaluated specifically for RF-based flood delineation. In this study, we investigate the consistency of RF feature-importance rankings in a binary flood-classification task primarily based on Synthetic Aperture Radar (SAR) imagery. The feature stack comprises 14 variables, including 9 SAR-based features, Sentinel-1 VV and VH polarizations and their temporal-change metrics which inform the flood extent identification, and 4 contextual features such as land cover and topographic indices which provide information on backscatter uncertainties. The classification task was conducted across 18 flood events spanning six distinct biomes: (1) Deserts and Xeric Shrublands, (2) Tropical and Subtropical Moist Broadleaf Forests, (3) Temperate Broadleaf and Mixed Forests, (4) Temperate Coniferous Forests, (5) Mediterranean Forests, Woodlands and Scrub, and (6) Temperate Grasslands, Savannas and Shrublands. Three feature-attribution methods were evaluated: (1) Shapley Additive exPlanations (SHAP) provides a game-theoretic framework for feature attribution and is widely recognized for its consistency and interpretability; (2) Mean Decrease in Impurity (MDI), computed during tree growth, is the most commonly used importance metric for RF models; (3) Permutation feature importance (MDA) offers a model-agnostic approach that assesses importance by measuring the reduction in model accuracy when feature values are randomly shuffled. Both feature cardinality and feature correlation, which bias the feature rankings for these algorithms in different ways, were considered during interpretation. All experiments were repeated across 10 independent iterations to account for random variability. We first examined feature-importance rankings independently across the three sub-sample studies within each biome to establish baseline intra-biome variability, followed by quantification of inter-biome variability to assess whether feature-importance patterns transfer across different environmental conditions. Preliminary results across select biomes indicate stable rankings for SAR-based features, with VV and VH event polarizations dominating the decision boundary, while contextual descriptors, particularly terrain indices such as Height Above the Nearest Drainage, exhibit greater variability both within and between biomes. Understanding the transferability of feature-importance patterns and feature stacks across biomes is critical for developing an RF-based flood-mapping pipeline that operates reliably under diverse environmental conditions worldwide and ultimately builds user trust in the resulting products.

How to cite: Havakhor, P., Hosch, P., and Dasgupta, A.: Cross-Biome Feature Importance Stability Analysis for SAR-based Flood Mapping with Random Forests, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1266, https://doi.org/10.5194/egusphere-egu26-1266, 2026.

EGU26-1859 | ECS | Posters on site | HS6.5

Detecting Waterlogging in Agricultural Fields in Denmark using High-Resolution PlanetScope Time Series 

Jasper Kleinsmann, Julian Koch, Stéphanie Horion, Gyula Mate Kovacs, and Simon Stisen

Waterlogging in agricultural fields is the condition of temporally inundated areas driven by extreme rainfall, rising groundwater or poor drainage, and has been identified as a major issue by Danish farmers. During the inundation period, plants are deprived of oxygen which negatively affects the root development and leads to decreased yields and grain quality. Additionally, these waterlogged areas are a large source of greenhouse gas (GHG) emissions. The issue is expected to exacerbate under current climate projections through wetter winters and rising groundwater levels in Denmark. Hence, an increased understanding of the spatio-temporal dynamics of waterlogging is required to future-proof the management strategies. The research goals are three-fold: (1) to optimise the detection of waterlogging, (2) to reveal inter- and intra-annual patters across Denmark and (3) to investigate the drivers of waterlogging such as climate, topography and bio-physical conditions. We aim to detect waterlogged areas through a deep learning semantic segmentation approach utilising multi-temporal PlanetScope imagery and nation-wide high resolution elevation data. This approach requires a manually delineated reference dataset to train, validate and test the model which needs to be well-balanced spatially, e.g. covering various soil types, and temporally, e.g. including various illumination conditions. Additionally, we will experiment with various model architectures, backbones and covariate combinations to optimise the segmentation performance. Initial tests using a UNET architecture and building upon a published reference dataset by Elberling et al. (2023), show promising results and lay the foundation for the upcoming model development and extension of the existing reference data.

 

Elberling, B. B., Kovacs, G. M., Hansen, H. F. E., Fensholt, R., Ambus, P., Tong, X., ... & Oehmcke, S. (2023). High nitrous oxide emissions from temporary flooded depressions within croplands. Communications Earth & Environment, 4(1), 463.

 

How to cite: Kleinsmann, J., Koch, J., Horion, S., Kovacs, G. M., and Stisen, S.: Detecting Waterlogging in Agricultural Fields in Denmark using High-Resolution PlanetScope Time Series, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1859, https://doi.org/10.5194/egusphere-egu26-1859, 2026.

EGU26-2995 | ECS | Orals | HS6.5

SaferSat: The Saferplaces’s  Operational Sentinel-1 Toolbox for Multi-Temporal Flood Extent Mapping, Water-Depth Estimation and Impact Assessment  

Saeid DaliriSusefi, Paolo Mazzoli, Valerio Luzzi, Francesca Renzi, Tommaso Redaelli, Marco Renzi, and Stefano Bagli

Operational flood intelligence for emergency response and insurance, providing a rapid overview of impacted land, population, and economic damages, requires mapping solutions that remain reliable under adverse observational conditions and across diverse landscapes. Although Sentinel-1 SAR provides consistent global, all-weather and day-and-night coverage, automated flood extraction is challenged by speckle noise, land-cover heterogeneity, and confusion between floodwater and permanent low-backscatter surfaces. These limitations highlight the need for approaches that exploit temporal backscatter changes while maintaining global robustness and computational efficiency.

We present SaferSat, a fully automated Sentinel-1 toolbox for flood-extent mapping, water-depth estimation, and impact assessment. SaferSat is part of SaferPlaces (saferplaces.co), a global Digital Twin platform for flood risk intelligence supporting emergency response and insurance applications. Central to the framework is Pr-RWU-Net (Progressive Residual Wave U-Net), a lightweight deep-learning model with 2.6 million trainable parameters, designed to detect flood-induced backscatter changes using VV-polarized SAR imagery. The model uses a three-channel input; pre-event VV, post-event VV, and their radiometric difference, enhancing inundation sensitivity while mitigating VH instability for global deployment.

SaferSat provides end-to-end processing: automated data retrieval, multi-date flood inference, and Maximum Flood Extent generation. To reduce SAR ambiguities, it generates auxiliary layers: a vegetation mask for SAR "blind spots" and a low-backscatter anomaly mask for permanent dark features. Flood extent layers are integrated with the FLEXTH model and GLO-30 or local high-resolution LiDAR DTMs for water-depth reconstruction. The system also analyzes acquisition patterns to predict short-term revisit opportunities. Impact assessment intersects flood extents with JRC GHS-POP and ESA WorldCover datasets.

The Pr-RWU-Net model was trained on the S1GFloods dataset, containing 5,360 paired pre- and post-event Sentinel-1 GRD images across 42 flood events from 2016–2022. Binary flood masks were generated via semi-automated thresholding and expert quality control. Evaluation on the test split achieved an IoU of 90.0%, F1-score 94.6%, Recall 95.6%, Precision 93.8%, and overall accuracy 96.6%.

Operational applicability was demonstrated on three 2025 flood events: Romania, Pakistan, and France. SaferSat flood extents closely matched SAR manual driven flood references (IoU 89–92%) and CEMS products (IoU 85–88%). Water-depth estimation against a reference hydrodynamic model yielded a MAE of 34–40 cm and correlation R of 0.78–0.82. For a 260 km² flood in Romania, the full processing chain completed in ~3 minutes on a standard CPU, demonstrating suitability for rapid, large-scale deployment.

SaferSat is available globally through SaferPlaces, supporting emergency response and insurance applications. Future developments aim to enhance SaferSat globally via integration of commercial satellite data to reduce revisit time and rapid hydrodynamic modeling to address radar limitations.

How to cite: DaliriSusefi, S., Mazzoli, P., Luzzi, V., Renzi, F., Redaelli, T., Renzi, M., and Bagli, S.: SaferSat: The Saferplaces’s  Operational Sentinel-1 Toolbox for Multi-Temporal Flood Extent Mapping, Water-Depth Estimation and Impact Assessment , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2995, https://doi.org/10.5194/egusphere-egu26-2995, 2026.

EGU26-3018 | Posters on site | HS6.5

Advancing Flood Forecasting in Large River Basins Using Multi-Mission Satellite Data: the EO4FLOOD project 

Angelica Tarpanelli and the EO4FLOOD Team

Floods are among the most destructive natural hazards worldwide, causing severe impacts on human health, ecosystems, cultural heritage and economies. Over the past decades, both developed and developing regions have experienced increasing flood-related losses, a trend that is expected to intensify under climate change due to shifts in precipitation patterns and the frequency of extreme events. In many large river basins, particularly in data-scarce regions, flood forecasting remains highly uncertain because of limited in situ observations and complex hydrological and hydraulic dynamics.

EO4FLOOD is an ESA-funded project aimed at demonstrating the added value of advanced Earth Observation (EO) data for improving flood forecasting at regional to continental scales. The project focuses on the integration of multi-mission satellite observations with hydrological and hydrodynamic modelling frameworks to support flood prediction up to seven days in advance, with an explicit treatment of uncertainty.

A key outcome of EO4FLOOD is the development of a comprehensive and openly available EO-based dataset designed to support flood modelling and forecasting studies. The dataset covers nine large and hydrologically complex river basins worldwide, selected to represent a wide range of climatic, physiographic and anthropogenic conditions, and characterized by limited or heterogeneous availability of ground-based observations. It integrates high-resolution satellite products from ESA and non-ESA missions, including precipitation, soil moisture, snow variables, flood extent, water levels and satellite-derived river discharge.

Within EO4FLOOD, these EO datasets are combined with hydrological and hydraulic models, enhanced by machine learning techniques, to improve flood prediction skill and to better quantify predictive uncertainty in data-scarce environments. The project also investigates the role of human interventions, such as reservoirs and land-use changes, in modulating flood dynamics across the selected basins.By making this multi-variable EO dataset publicly available, EO4FLOOD aims to support the broader hydrological community in testing, benchmarking and developing flood modelling and forecasting approaches in challenging large-basin settings. The project provides a unique opportunity to explore the potential and limitations of EO-driven flood forecasting and contributes to advancing the use of satellite observations for global flood risk assessment and management.

How to cite: Tarpanelli, A. and the EO4FLOOD Team: Advancing Flood Forecasting in Large River Basins Using Multi-Mission Satellite Data: the EO4FLOOD project, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3018, https://doi.org/10.5194/egusphere-egu26-3018, 2026.

            Water security in the Chi River Basin is critical for the agricultural economy and ecosystem stability of Yasothon Province, Thailand. However, effective spatiotemporal monitoring of water surface dynamics is frequently hindered by persistent cloud cover during the monsoon season, limiting the utility of traditional optical remote sensing. This study addresses this challenge by developing a robust Multi-Sensor Deep Learning Fusion system that integrates Synthetic Aperture Radar (SAR) and optical satellite imagery to ensure continuous observation capabilities.

            We employ a U-Net convolutional neural network architecture, selected for its high boundary precision and efficiency with limited training datasets. The model is trained on a fused six-channel input configuration, combining Sentinel-1 SAR data (weather-independent) with Sentinel-2 optical bands (RGB), augmented by the Normalized Difference Water Index (NDWI) and Normalized Difference Vegetation Index (NDVI). This multi-modal approach enhances feature extraction, allowing for the accurate differentiation of open water from floating vegetation and flooded agricultural lands in complex transition zones.

            The study analyzes the hydrological cycle of 2022, capturing distinct drought, flood, and post-flood conditions. To ensure hydrological validity, the model’s segmentation outputs are not merely visually assessed but are quantitatively validated against ground-truth water level data from the E.20A gauge station in Kham Khuean Kaeo District. By establishing a precise Stage-Area Relationship, this research demonstrates a scalable, cost-effective framework for flood risk assessment and water capital estimation, offering a resilient solution for river basin management in cloud-prone tropical regions.

How to cite: Pruekthikanee, P.: Multi-Sensor Deep Learning Fusion for Spatiotemporal Water Surface Monitoring in the Yasothon Province's Chi River Basin, Thailand, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4154, https://doi.org/10.5194/egusphere-egu26-4154, 2026.

EGU26-5752 | ECS | Orals | HS6.5

Satellite-Enhanced Flood Modelling for the Niger River Basin using a Synergy of Hydrological Modelling and Earth Observation Data 

Shima Azimi, Alexandra Murray, Connor Chewning, Cecile Kittel, Henrik Madsen, Fan Yang, Maike Schumacher, and Ehsan Forootan

Accurate water cycle representation in data-scarce and flood-prone regions like the Niger River Basin demands stronger integration between remote sensing and hydrological modelling. Spanning ten water-stressed nations, this basin faces critical challenges under climate change, requiring robust water-budget assessments to guide resilience strategies. We employ DHI’s Global Hydrological Model (DHI-GHM) to simulate key hydrological components of the regional water cycle. Model outputs for surface and root-zone soil moisture (SSM and R-ZSM) and terrestrial water storage (TWS) are systematically compared against satellite observations (GRACE/GRACE-FO and multiple soil moisture products) to identify discrepancies and enhance the understanding of regional hydrological behavior. A near real-time SSM data assimilation scheme is implemented to enhance spatiotemporal accuracy of surface and top-soil interactions, particularly beneficial in the flood-sensitive Inner Niger Delta. Post-assimilation hydrological outputs are coupled with the CaMa-Flood surface hydraulic model to simulate inundation dynamics, enabling improved flood prediction and supporting risk management. Finally, we pursue two-way coupling of hydrological and hydrodynamic models by integrating river flow–storage feedbacks to advance flood forecasting and sustainable water-resources planning. 

How to cite: Azimi, S., Murray, A., Chewning, C., Kittel, C., Madsen, H., Yang, F., Schumacher, M., and Forootan, E.: Satellite-Enhanced Flood Modelling for the Niger River Basin using a Synergy of Hydrological Modelling and Earth Observation Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5752, https://doi.org/10.5194/egusphere-egu26-5752, 2026.

EGU26-5862 | ECS | Orals | HS6.5

Refining global wetland characterization using an unsupervised, wetness-based dynamic framework 

Yang Li, Nandin-Erdene Tsendbazar, Kirsten de Beurs, Lassi Päkkilä, and Lammert Kooistra

Existing global wetland datasets and monitoring approaches emphasizepersistent inundation, while intermittent inundation and waterlogged states—especially where vegetation is present—are underrepresented or of lower accuracy. This leads to inaccurate estimates of greenhouse gas emissions from carbon-rich systems (e.g., peatlands). Meanwhile, the predominance of annual mapping limits the capture of intra-annual variability, further reinforcing these inaccuracies and obscuring sub-seasonal disturbances from human activities (e.g., shifts in rice-cropping intensity). This study presents an unsupervised, wetness-driven framework for improving global wetland monitoring that leverages earth observation data streams. For framework development, the OPtical TRApezoid Model is applied to Harmonized Landsat-Sentinel imagery to retrieve surface wetness, followed by wetland delineation using a scene-adaptive grid-based thresholding algorithm. This framework is applied to 824 globally distributed 0.1° grid cells encompassing 9,781 land-cover-labeled sites and 134 sites with daily wet–dry labels across 28 Ramsar wetlands, and validated for spatial delineation, thematic, and temporal accuracy. Comparative analysis employs Dynamic World, the first global 30 m wetland map with a fine classification system (GWL_FCS30), and the modified Dynamic Surface Water Extent algorithm (DSWE). Our framework achieved moderate spatial delineation accuracy with F1 of 0.64 (recall 0.75, precision 0.56), comparable in F1 to Dynamic World and with higher recall than DSWE and GWL_FCS30. It delivered the highest temporal accuracy (F1 0.72; precision 0.81; recall 0.64) and improved thematic accuracy for vegetated wetland, reducing omission with modest commission. The proposed wetland monitoring framework enables more accurate targeted policy interventions.

How to cite: Li, Y., Tsendbazar, N.-E., de Beurs, K., Päkkilä, L., and Kooistra, L.: Refining global wetland characterization using an unsupervised, wetness-based dynamic framework, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5862, https://doi.org/10.5194/egusphere-egu26-5862, 2026.

EGU26-6114 | ECS | Orals | HS6.5

Evidential Deep Learning for Uncertainty-Aware Global Flood Extent Segmentation 

Chi-ju Chen and Li-Pen Wang

Flood extent mapping from satellite imagery plays a critical role in disaster response and flood risk management, particularly as flood events become more frequent and severe under a changing climate. At its core, the task involves classifying each pixel in an optical satellite image as flooded or non-flooded. Recent deep learning-based segmentation models have demonstrated strong performance at the global scale. However, despite their accuracy, most existing approaches provide deterministic predictions and offer limited information on the reliability of individual pixel-level outputs. This lack of uncertainty information constrains their operational applicability, especially in high-risk scenarios where models may exhibit overconfident but incorrect predictions.

To address this limitation, we extend a global flood extent segmentation framework by explicitly incorporating uncertainty quantification. Specifically, an Evidential Deep Learning (EDL) approach is integrated into a UNet++ architecture within the ml4floods framework, enabling simultaneous prediction of flood extent and associated pixel-wise uncertainty. Within the EDL formulation, network outputs are interpreted as evidence and parameterised using a Beta distribution, providing a principled estimate of predictive uncertainty. Furthermore, total uncertainty is decomposed into aleatoric and epistemic components, allowing clearer interpretation of whether uncertainty arises from data ambiguity or from limited model knowledge.

The proposed approach is evaluated using the extended WorldFloods global flood dataset. Preliminary results indicate that the EDL-enhanced model maintains promising segmentation performance while producing informative uncertainty maps. Elevated uncertainty is consistently observed in misclassified regions and along land-water boundaries, where optical signals are inherently ambiguous. These results demonstrate that uncertainty estimates offer valuable insight into model reliability and support operational decision-making by highlighting areas that require closer inspection. In practice, uncertainty-guided triage can help prioritise expert review and resource allocation, focusing attention on regions where decision risk is highest.

How to cite: Chen, C. and Wang, L.-P.: Evidential Deep Learning for Uncertainty-Aware Global Flood Extent Segmentation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6114, https://doi.org/10.5194/egusphere-egu26-6114, 2026.

EGU26-6180 | ECS | Orals | HS6.5

 The capabilities of virtual gauging stations in satellite monitoring of water bodies 

Ildar Mukhamedjanov and Gulomjon Umirzakov

Remote sensing technologies provide effective tools for monitoring and assessing the state of inland water bodies, enabling extraction of various hydrological parameters from satellite observation. Central Asian and some African countries are currently implementing practical programs aimed at mitigating water scarcity and improving the management of transboundary water resources. Rivers and their tributaries flowing across national boundaries require continuous monitoring to support early warning of droughts and floods at the basin scale.

Conventional ground-based hydrological stations are traditionally used to measure water level, estimate daily river discharge, and support hydrological forecasting. However, limitations related to accessibility, data-sharing restrictions, and the high cost of installation and maintenance often constrain their spatial coverage and long-term operation.  Virtual gauging station (VGS) represents a complementary remote-sensing approach, providing time series derived from the long-term satellite image archives. A VGS is defined as a free-shaped polygon on the map used to analyze data within the borders of this polygon and collect observations based on the requirements. Currently, VGS applications primarily rely on optical satellite imagery from Sentinel-2, Landsat-4, -5, -7, -8, -9 missions to estimate water surface area (WSA) using spectral water index (MNDWI, AWEI or AWEIsh). Variations in WSA serves as a proxy for surface water availability and river dynamics. 

In addition, VGS can be used to enrich satellite altimetry-based water level (H) time series. For this purpose, the VGS polygon is calibrated using reference altimetric observations obtained from open-access data source (e.g. SDSS, DAHITI, Hydroweb). Calibration involves estimating the parameters of a regression model describing the functional relationship between water level and water surface area.  The resulting values can finally be integrated into hydrological models to support short-term river discharge forecasting. Thus, VGS provides continuous hydrological information independent of ground-based measurements, while optional validation against in-situ observations allows for the assessment of the model uncertainty.  Based on the experimental analysis, optimal placement of VGS polygons is recommended dynamically active river sections that account for annual riverbed displacement, as well as in river reaches located near satellite altimeter ground tracks to improve calibration accuracy.

The experiments demonstrated that correlation between ground truth and forecasted water level values is upper 0,85 and mean absolute error is lower than 0,3 m. The following result has been obtained using linear regression which shows that application of more complex forecasting models could significantly improve the results.

How to cite: Mukhamedjanov, I. and Umirzakov, G.:  The capabilities of virtual gauging stations in satellite monitoring of water bodies, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6180, https://doi.org/10.5194/egusphere-egu26-6180, 2026.

EGU26-6408 | ECS | Posters on site | HS6.5

Multisensor Ensemble Mapping of Sub-hectare Ephemeral Surface Water in Kenyan ASALs 

James Muthoka, Pedram Rowhani, Chloe Hopling, Omid Memarian Sorkhabi, and Martin Todd

Ephemeral pans and seasonal ponds in arid and semi-arid lands supply critical water for pastoral and ecological systems, yet are not routinely monitored due to their small size, highly dynamic and spectral confusion with vegetation and shadows. We present and evaluate a multisensor mapping approach to detect sub-0.5 ha surface water bodies and quantify their linkage to rainfall variability to inform decision making.

Our approach fuses Sentinel-1 SAR, Sentinel-2 optical indices and DEM derived covariates within an ensemble classifier (voting of Random Forest, Gradient Boosting, and Decision Tree models). Predictive uncertainty is mapped using ensemble agreement and class probabilities, and we compare SAR-only, optical-only, terrain-only, and fused configurations. Additionally, rain and ephemeral surface water dynamics are modelled using generalised additive models with CHIRPs  and local rain gauge observations to test the lagged relationships in monthly water area anomalies.

Results show the fused model achieves an overall accuracy of 85%, outperforming Sentinel-1, and Sentinel-2 (78% and 72%, respectively). Generalised additive models explain 62% of variance in monthly water area anomalies, with a strong response at 1-3 month lags. These results show multisensor fusion with  quantified uncertainty improves detection of ephemeral surface water and enables estimation of rainfall thresholds and lagged dynamics relevant to pastoral water planning and targeted anticipatory action interventions.

How to cite: Muthoka, J., Rowhani, P., Hopling, C., Memarian Sorkhabi, O., and Todd, M.: Multisensor Ensemble Mapping of Sub-hectare Ephemeral Surface Water in Kenyan ASALs, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6408, https://doi.org/10.5194/egusphere-egu26-6408, 2026.

EGU26-6586 | ECS | Posters on site | HS6.5

Do Geospatial Foundation Models Improve SAR-Based Flood Mapping?  

Antara Dasgupta and Moetez Zouaidi

Accurate and timely flood delineation is a cornerstone of disaster response and hydrological risk management. Synthetic Aperture Radar (SAR) is uniquely suited to this task because it operates independently of cloud cover and illumination, yet its interpretation remains challenging due to speckle, terrain effects, vegetation scattering, and ambiguities between flooded and permanent water as well as shadows and smooth surfaces such as tarmac. While deep learning has substantially advanced SAR-based flood segmentation, most existing models are trained from scratch and often struggle to generalize across regions and flood regimes. Recently, geospatial foundation models (GFMs) pretrained on massive satellite archives have shown promise, but their benefits for SAR-based flood mapping remain insufficiently quantified. This paper presents a controlled, large-scale global scale evaluation and benchmarking of a vision-transformer based GFM (NASA IBM Prithvi) against two task-specific segmentation architectures, the SegFormer (hierarchical transformer) and the commonly used U-Net (convolutional neural network), including lightweight variants, for post-event SAR-based flood mapping. All models were trained and evaluated under a standardized pipeline that explicitly addresses extreme class imbalance via stratified negative sampling and weighted loss functions. Training and validation used the expert-annotated Kuro Siwo dataset (43 flood events, 67,490 Sentinel-1 VV/VH tiles), while generalization is assessed on both the in-distribution Kuro Siwo test set and the out-of-distribution Sen1Floods11 hand labelled benchmark dataset. Results show that stratified negative sampling (controlling how many background-only tiles are shown to the model in each training epoch) increases precision by approximately 6% and mean Intersection-over-Union (mIoU) by about 7% relative to no sampling, while stabilizing training loss dynamics. On the in-distribution data, all architectures reach similar performance (mIoU ≈ 0.82), indicating that well-designed task-specific models remain competitive with GFMs. However, under out-of-distribution conditions, the foundation model Prithvi (mIoU 0.768) closely matches the performance of the SegFormer (mIoU 0.772) and clearly outperforms the U-Net (mIoU 0.712), highlighting the robustness of transformer-based representations when transferring across datasets. Pretraining on optical imagery yields only modest gains for SAR (+3.4% mIoU), suggesting that architectural inductive biases and data handling matter more than cross-modal pretraining. Notably, lightweight GFM variants achieve comparable accuracy with up to 94% fewer parameters, demonstrating strong potential for operational deployment. Scene-level analysis reveals that CNNs suppress scattered false alarms due to the neighborhood contextualization but miss large, continuous floods, while transformers preserve spatial coherence yet overpredict along complex boundaries and scattered surface water ponding, especially near permanent water bodies. Findings demonstrate that while SAR-based flood mapping accuracy requires a combination of appropriate model architectures and class imbalance-aware training, rather than foundation-scale pretraining alone. However, for spatial and statistical transfer to out of distribution datasets, GFMs offer substantial advantages and provide above-average performance for unseen cases, even without localized fine-tuning.

How to cite: Dasgupta, A. and Zouaidi, M.: Do Geospatial Foundation Models Improve SAR-Based Flood Mapping? , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6586, https://doi.org/10.5194/egusphere-egu26-6586, 2026.

EGU26-6617 | ECS | Posters on site | HS6.5

SARFlood: A Web-Based, Cloud-Native Platform for Automated and Optimized ML-based SAR Flood Mapping    

Patrick Wilhelm, Paul Hosch, and Antara Dasgupta

Synthetic Aperture Radar (SAR) imagery offers weather-independent observation capabilities critical for monitoring flood events. However, SAR-based flood detection workflows typically require specialized software, local computational resources, and expert knowledge in remote sensing. This work presents SARFlood, a web-accessible application that automates the complete SAR flood detection pipeline using the OpenEO platform. SARFlood is built on a Flask backend architecture designed for accessibility and reproducibility. Users interact with the system through a web interface that guides them through case study creation, including Area of Interest (AOI) definition via shapefile upload, event date specification, and optional ground truth data integration. The application implements OpenEO OAuth 2.0 authentication using the device code flow, enabling secure access to the Copernicus Data Space Ecosystem (CDSE) backend without requiring users to manage API credentials locally. Session-based project management allows users to track processing progress in real-time through a status reporting system that monitors each pipeline stage. Data acquisition is performed server-side via OpenEO, while feature engineering processors execute locally. The data acquisition module fetches multiple data sources through a unified OpenEO interface: pre-event and post-event Sentinel-1 VV and VH imagery, Digital Elevation Models (DEM) with automatic source fallback (FABDEM, Copernicus 30m/90m), and ESA WorldCover land cover classification. The OpenStreetMap water body features and the FathomDEM are acquired via their own APIs/websites. A caching system prevents redundant API calls for previously acquired datasets, significantly reducing processing time for iterative analyses, while keeping licensing in mind so only users who are logged in and have the according license will be able to access the cached files. The processing pipeline computes a comprehensive feature stack for flood detection. SAR derivatives include intensity bands, VV/VH polarization ratios, and change detection metrics computed in decibel space to enhance flood signal discrimination. Topographic features encompass slope and Height Above Nearest Drainage (HAND) derived from the DEM, as key indicators of flood susceptibility. Flow direction calculations use an expanded bounding box to determine the extended HAND computation domain to address edge artifacts, finally cropped to the original AOI during band compilation, ensuring computationally efficient and accurate flow routing. Additionally, stream burning is implemented to improve drainage network delineation. Further, contextual features include Euclidean Distance to Water and rasterized land cover classification. Users can currently upload ground truth shapefiles (e.g., Copernicus EMS), which are automatically rasterized and compiled into the output stack, enabling supervised classification workflows.  

SARFlood includes integrated sampling and training modules. Multiple strategies such as Simple Random, Stratified, Generalized Random Tessellation Stratified, and Systematic Grid sampling are supported. The training module implements Random Forest classification with Leave-One-Group-Out Cross-Validation across multiple case studies, hyperparameter optimization via Bayesian search, and feature importance assessment through Mean Decrease Impurity, permutation importance, and SHAP values. The platform-, data- and model-agnostic design principles used in developing SARFlood, support open science and FAIR practices in the geoscience community. By combining web accessibility with robust feature engineering and machine learning integration, SARFlood provides researchers with a reproducible platform for generating uncertainty-aware flood labels lowering barriers to use. 

How to cite: Wilhelm, P., Hosch, P., and Dasgupta, A.: SARFlood: A Web-Based, Cloud-Native Platform for Automated and Optimized ML-based SAR Flood Mapping   , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6617, https://doi.org/10.5194/egusphere-egu26-6617, 2026.

EGU26-7132 | ECS | Orals | HS6.5

Monitoring Freshwater Bodies over the Past 40 Years Using Synthetic Monthly Sentinel-2 MSI Imagery  

Federica Vanzani, Patrice Carbonneau, Simone Bizzi, Martina Cecchetto, and Elisa Bozzolan

In the last decade rapid advancements in remote sensing have opened new frontiers in our ability to monitor freshwater bodies dynamics at the global scale. Most works have taken advantage of the long time series of Landsat constellations (30 m resolution) relying on spectral indices to identify water. Recently, much progress has also been made in the development and use of deep learning models capable of explicit semantic classification of river water, lake water and sediment bars, based on Sentinel-2 (S2) MSI imagery (10 m resolution). In this work, we present an approach that seeks to extend these existing, trained, fluvial landscape classification models to Landsat data in order to observe long-term water and morphological shifts in rivers and lakes. Rather than explicitly re-training the models with Landsat data and labour-intensive manual label data, we apply a domain transfer approach to generate synthetic S2 MSI imagery from Landsat inputs. This approach has the advantage that the training of deep learning domain transfer models only requires synchronous Landsat and Sentinel data and thus obviates the need for manual labels.

The results show that, when using these synthetic images, river water, lake water and sediment bars are classified with an F1 score of 0.8, 0.94, 0.65 respectively, which represents a decrease of ca. 10% for river water and 20% for sediment with respect to real S2 imagery. By adopting this integrated approach, we are therefore able to monitor, for the first time, lake water, river water and sediment bars at 10 m resolution, over a 40-year period, integrating both synthetic S2 and real S2 acquisitions through a single, fluvial landscape segmentation model. Classification obtained from median monthly images can then be aggregated at the yearly or multi-yearly scale to delineate river or lake water fluctuations, and active channels (river water plus sediment bars) trajectories, from specific freshwater bodies to the global scale.

How to cite: Vanzani, F., Carbonneau, P., Bizzi, S., Cecchetto, M., and Bozzolan, E.: Monitoring Freshwater Bodies over the Past 40 Years Using Synthetic Monthly Sentinel-2 MSI Imagery , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7132, https://doi.org/10.5194/egusphere-egu26-7132, 2026.

EGU26-7320 | ECS | Posters on site | HS6.5

Evaluating multimodal optical and SAR learning strategies for flood and surface water delineation 

jiayin xiao, zixi li, and fuqiang tian

Flood and surface water mapping from satellite observations remains challenging due to the complementary yet heterogeneous characteristics
of optical and synthetic aperture radar (SAR) data. While deep learning has achieved promising results, existing studies are often evaluated on
isolated datasets or focus on a single modality, limiting their comparability and operational relevance. In this study, we conduct a large-scale and systematic evaluation of optical, SAR, and combined optical–SAR learning strategies for flood and surface water mapping across multiple public satellite benchmarks. Using a common training and evaluation protocol, we compare lightweight convolutional networks and large pretrained vision models under single-modality and multimodal settings. The analysis reveals that attention-based multimodal fusion consistently improves water delineation accuracy on most datasets, while model capacity and preprocessing choices play a critical role in balancing missed detections and false alarms. On global-scale benchmarks, moderately sized backbones coupled with dedicated fusion mechanisms achieve robust performance without relying on extremely large models.These findings provide practical guidance for selecting architectures and fusion strategies in operational flood mapping and establish a reproducible benchmark for future optical and SAR studies.

How to cite: xiao, J., li, Z., and tian, F.: Evaluating multimodal optical and SAR learning strategies for flood and surface water delineation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7320, https://doi.org/10.5194/egusphere-egu26-7320, 2026.

EGU26-7998 | Orals | HS6.5

Ten years of floods across Europe mapped from space with reconstructed water depths  

Andrea Betterle and Peter Salamon

Floods are among the most deadly and destructive natural disasters. Improving our understanding of large-scale flood dynamics is crucial to mitigating their dramatic consequences. Unfortunately, systematic observation-based datasets—especially featuring flood depths—have been lacking.

This contribution presents advancements in developing an unprecedented catalogue of satellite-derived flood maps across Europe from 2015 onwards. Results are based on the systematic identification of floods in the entire Sentinel-1 archive at 20 m spatial resolution as provided by the Global Flood Monitoring component of the Copernicus Emergency Management Service. Using a novel algorithm that accounts for terrain topography, flood maps are enhanced and provided with water depth estimates—a critically important information for flood impact assessments.

The resulting dataset represents a significant step towards the creation of a global flood archive. It provides new tools for interpreting flood hazards on large scales, with substantial implications for flood risk reduction, urban development planning, and emergency response.

How to cite: Betterle, A. and Salamon, P.: Ten years of floods across Europe mapped from space with reconstructed water depths , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7998, https://doi.org/10.5194/egusphere-egu26-7998, 2026.

EGU26-8292 | Posters on site | HS6.5

Modelling wetland resilience to climate change and anthropogenic impacts. 

Patricia Saco, Rodriguez Jose, Breda Angelo, Eric Sandi, and Steven Sandi

Coastal wetlands provide a wide range of ecosystem services, including shoreline protection, attenuation of storm surges and floods, water quality improvement, wildlife habitat and biodiversity conservation. These ecosystems have been observed to sequester atmospheric carbon dioxide at rates significantly higher than many other ecosystems, positioning them as promising nature-based solutions for climate change mitigation.  However, projections of coastal wetland conditions under sea-level rise (SLR) remain highly variable, owing to uncertainties in environmental factors as well as the necessary simplifications embedded within the wetland evolution modelling frameworks. Assessing wetland resilience to rising sea levels and the effect of anthropogenic activities is inherently complex, given the uncertain nature of key processes and external influences. To enable long-term simulations that span extensive temporal and spatial scales, models must rely on a range of assumptions and simplifications—some of which may significantly affect the interpretation of wetland resilience.

 

Here we present a novel eco-hydro-geomorphological modelling framework to predict wetland evolution under SLR. We explore how accretion and lateral migration processes influence the response of coastal wetlands to SLR, using a computational framework that integrates detailed hydrodynamic and sediment transport processes. This framework captures the interactions between physical processes, vegetation, and landscape dynamics, while remaining computationally efficient enough to support simulations over extended timeframes. We examine several common simplifications employed in models of coastal wetland evolution and attempt to quantify their influence on model outputs. We focus on simplifications related to hydrodynamics, sediment transport, and vegetation dynamics, particularly in terms of process representation, interactions between processes, and spatial and temporal discretisation. Special attention is given to identifying modelling approaches that strike a balance between computational efficiency and acceptable levels of accuracy. We will present recent model results to assess the resilience of coastal wetland to SLR on several sites around the world and will discuss new results to assess the effect of human interventions and infrastructure on wetland resilience.

How to cite: Saco, P., Jose, R., Angelo, B., Sandi, E., and Sandi, S.: Modelling wetland resilience to climate change and anthropogenic impacts., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8292, https://doi.org/10.5194/egusphere-egu26-8292, 2026.

EGU26-9354 | ECS | Orals | HS6.5

L-band InSAR to complement SAR inundation mapping under vegetation 

Clara Hübinger, Etienne Fluet-Chouinard, Daniel Escobar, and Fernando Jaramillo

Wetland inundation dynamics are key for understanding flood regulation, ecosystem functioning and greenhouse gas emissions. Synthetic Aperture Radar (SAR) can map water extent independent of cloud cover and can partly penetrate vegetation, particularly at L-band. Many SAR inundation products rely primarily on intensity thresholding and indicators such as specular reflection and double-bounce scattering. However, these approaches can underestimate inundation extent in densely vegetated wetlands where volume scattering can obscure the water signal. Here we demonstrate how L-band interferometric SAR (InSAR) can complement intensity-based inundation mapping under vegetation by exploiting phase differences between repeat SAR acquisitions. Using ALOS PALSAR-1 and PALSAR-2, together providing a nearly two-decade observational archive, we show that L-band InSAR can capture inundation dynamics in tropical floodplain wetlands, such as the Atrato floodplain (Colombia) and Amazon várzea floodplains (e.g., along the Río Pastaza). In the Atrato floodplain, the InSAR-derived flooded vegetation extent shows pronounced seasonal variability, ranging from ~500 to >1500 km² during 2007–2011. Comparison with existing L-band SAR inundation products yields ~70% overall agreement, while InSAR consistently detects broader inundated extents in densely vegetated floodplain areas where intensity-based thresholding underestimates inundation. This complementarity among methodologies is particularly relevant for inundation extent data products from the NASA–ISRO NISAR mission, which are expected to rely largely on SAR backscatter thresholding. Our results highlight the value of integrating InSAR-derived information to strengthen wetland inundation monitoring under vegetated canopies.

How to cite: Hübinger, C., Fluet-Chouinard, E., Escobar, D., and Jaramillo, F.: L-band InSAR to complement SAR inundation mapping under vegetation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9354, https://doi.org/10.5194/egusphere-egu26-9354, 2026.

EGU26-9758 | ECS | Orals | HS6.5

Hydrologically-Informed DTM Super-Resolution for Rapid Flood Depth Estimation 

Sandro Groth, Marc Wieland, Christian Geiß, and Sandro Martinis
Reliable estimation of flood depths from satellite-derived inundation extent information critically depends on the spatial resolution and hydrological consistency of the underlying digital terrain model (DTM). Accurate, very high–resolution DTMs are typically not publicly available, difficult to access within the time constraints of rapid mapping, and lack consistent coverage. Although open-access DTMs such as the Forest and Buildings removed Copernicus DEM (FABDEM) provide global coverage, their coarse spatial resolution often fails to represent important small-scale terrain features that control flow paths, slopes, and local water accumulation. To address these limitations, this study proposes a deep learning framework for DTM super-resolution that combines low-resolution DTMs with optical satellite imagery by integrating hydrological knowledge into the training process to force the reconstruction of relevant topographic features for improved flood inundation depth estimation.

The proposed approach employs a residual channel attention network (RCAN) enhanced with optical satellite imagery as auxiliary input to upscale low-resolution terrain data. Central to the methodology is a collaborative hydrologic loss function that guides network optimization beyond elevation-based accuracy. In addition to the mean absolute elevation error (MAE), the loss integrates slope deviation and flow direction disagreement to focus the learning on the reconstruction of terrain features that are directly relevant for hydrologic applications.

Unlike other super-resolution approaches, which are often using downscaled versions of the low-resolution inputs to learn super-resolved DTMs, the proposed framework was trained on a growing set of aligned patches of real-world globally available low-resolution elevation data, optical satellite imagery, and high-resolution reference DTMs derived from airborne LiDAR. Model performance is evaluated against conventional interpolation and standard super-resolution baseline architectures, including convolutional neural networks (CNN) as well as geospatial foundation models (GFM). To assess the practical impact on flood mapping, the super-resolved DTMs are tested on a set of real-world flood events in Germany by using the well-known Flood Extent Enhancement and Water Depth Estimation Tool (FLEXTH) to derive inundation depth metrics.

Results show that integrating DTMs derived using hydrologically guided super-resolution into flood depth tools can lead to more accurate flood depth estimates compared to low-resolution or other super-resolved inputs. The added hydrologic loss significantly improves the preservation of slopes and flow directions while maintaining elevation accuracy.

Overall, the presented framework offers a method to generate hydrologically meaningful high-resolution DTMs from globally available low-resolution inputs to benefit flood depth estimation in areas, where no high-resolution terrain information is available.

How to cite: Groth, S., Wieland, M., Geiß, C., and Martinis, S.: Hydrologically-Informed DTM Super-Resolution for Rapid Flood Depth Estimation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9758, https://doi.org/10.5194/egusphere-egu26-9758, 2026.

Flash flood disasters have increased by more than 50% in the first 20 years of the 21st century compared to the last 20 years of the 20th century. Monitoring and understanding flood events might lead to better mitigation of this natural hazard. Using SAR and SAR interferometry (InSAR) proved to be a useful tool for mapping flooded areas due to the lower backscatter or decorrelation of the SAR signal in an open-water environment. In Arid regiem, flash flood water is rapidly drained by evaporation or percolation, often before the satellite image is acquired. To overcome this challenge, we propose in this study to use the InSAR coherency loss, created by surface changes during a flash-flood, to map the runoff path and utilize it to quantify peak discharge (Qmax).

We focus on the Ze’elim alluvial fan along the western shore of the Dead Sea, Israel, an arid area affected by seasonal flash floods a few days a year. We use 34 interferograms of X-band (COSMO-SkyMed/TerraSAR-X) SAR data, covering 25 runoff events between 2017 and 2021, and upstream hydrological gauge data. To consider the natural decorrelation processes, we calculate a normalized coherence (ϒn) term, using the average coherence of the study area and the average coherence of a stable reference area, identified by differential LiDAR measurements.

We find a strong correlation between gn and the logarithm of the peak discharge (Qmax). However, the method is limited by a minimal peak discharge—where energy is too low to change the surface—and maximal total water volume—where decorrelation is saturated. The method may provide tools for reconstructing runoff data in arid areas where historical SAR data is available, and for monitoring in difficult access areas or where hydrological stations are sparse or damaged.

How to cite: Nof, R.: Estimating Flash Flood Discharge in Arid Environments Using InSAR Coherence: A Case Study of the Ze’elim Fan, Dead Sea, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11948, https://doi.org/10.5194/egusphere-egu26-11948, 2026.

EGU26-12249 | Orals | HS6.5 | Highlight

Lessons Learned from Remote Sensing of River Ice for Flood Early Warning 

Arjen Haag, Tycho Bovenschen, Elena Vandebroek, Athanasios Tsiokanos, Ben Balk, and Joost van der Sanden

Rivers in regions with cold winters can seasonally freeze up. River ice breakup and freeze-up processes can lead to river ice jams, which are a major contributor to flood risk in cold regions (across most of the high latitudes of the northern hemisphere). In Canada, satellite remote sensing is used across the country to provide timely information on the status of river ice. Methods and algorithms to classify various stages of river ice from the Radarsat Constellation Mission (RCM) are available, but the operational implementation of these, especially the integration into larger flood forecasting and early warning systems, requires specific expertise, software and computational resources, and comes with its own set of challenges. In collaboration with various agencies across Canada we have set up operational monitoring systems with the purpose of assisting the daily tasks of forecasters on duty. These have been used in practice over multiple ice breakup and freeze-up seasons, which has highlighted both their usefulness and shortcomings. We will focus on various aspects of such a system and share lessons learned on its design, setup and operational use, as well as a framework to analyse various factors relevant for operational monitoring purposes (e.g. spatiotemporal coverage and latency of the data, critical elements in the support of decision-making relating to floods). In this, we do not shy away from problems and pitfalls, so that others can learn from these. While various challenges remain, this work is a good example of the value in the joint engagement of applied science and end users.

How to cite: Haag, A., Bovenschen, T., Vandebroek, E., Tsiokanos, A., Balk, B., and van der Sanden, J.: Lessons Learned from Remote Sensing of River Ice for Flood Early Warning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12249, https://doi.org/10.5194/egusphere-egu26-12249, 2026.

EGU26-13343 | Posters on site | HS6.5

Operational, national-scale monitoring of river trajectories using satellite imagery  

Elisa Bozzolan, Marco Micotti, Elisa Matteligh, Alessandro Piovesan, Federica Vanzani, Patrice Carbonneau, and Simone Bizzi

The global degradation of river ecosystems and the growing impacts of flood hazards have highlighted limitations in current river management approaches. In Europe, the Water Framework and Flood Directives promote integrated, catchment-scale assessments of hydromorphological conditions and flood risk. Such integration is essential for sustainable management. Planform dynamics and river bed aggradation/incision, for example, can modify channel conveyance and compromise flood mitigation measures, whereas granting more space to rivers can both enhance ecological quality and reduce flood peaks.

In this context, the availability of long-term satellite archives and advances in computational and machine-learning methods enable large-scale, high spatiotemporal resolution monitoring of large and medium river systems. However, despite this potential, the operational adoption of satellite-based river monitoring remains limited due to data complexity, interdisciplinary requirements, and the lack of harmonised computational infrastructures.

Thanks to a collaboration between industry, public institutions and the university, we developed a methodology to systematically map monthly water channel, channel width, sediment bars and vegetation dynamics, testing the results on the full archive of Sentinel-2 (10 m resolution) for medium-large Italian rivers (active channel > 30m - i.e. 3 Sentinel-2 pixels). In this talk, I will outline the applied methodology, discuss its applicability at national scale with Sentinel-2 data, and show how the generated products can better inform river habitat mapping, river conservation practices, and flood risk assessments by supporting consistent national scale geomorphic trajectories identification.

How to cite: Bozzolan, E., Micotti, M., Matteligh, E., Piovesan, A., Vanzani, F., Carbonneau, P., and Bizzi, S.: Operational, national-scale monitoring of river trajectories using satellite imagery , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13343, https://doi.org/10.5194/egusphere-egu26-13343, 2026.

Flood inundation mapping has become increasingly critical as climate change intensifies the frequency and severity of flooding worldwide, amplifying risks to populations, infrastructure, and ecosystems. Recent advances in Earth Observation (EO) have shown unprecedented opportunities to monitor flood dynamics across large spatial scales.. However, significant challenges remain due to the limitations of single-sensor approaches. While multispectral imagery provides rich semantic information, it is frequently constrained by cloud cover during flood events. Conversely, Synthetic Aperture Radar (SAR) offers all-weather capability but suffers from signal ambiguity in complex terrains and urban environments. Effectively integrating these heterogeneous modalities therefore remains a challenge, particularly with limited labelled flood event data.

In this study, we propose a deep learning-based cross-modal fusion framework that leverages the representational capacity of Remote Sensing Foundation Models (RSFMs). High-level feature embeddings are extracted from Sentinel-1 and Sentinel-2 multispectral imagery by initializing modality-specific encoders with pretrained weights from state-of-the art multi-modal foundation models, providing a robust and semantically aligned feature space despite limited task-specific training data 

To integrate the multi-modal representations, we adopt a Gated Cross-Modal Attention mechanism, which adaptively modulates the information flow from each modality based on their observation reliability. Specifically, the model is trained to prioritise SAR features to ensure spatial continuity under cloud-obscured conditions, while simultaneously leveraging richer optical semantics to disambiguate SAR signals, correcting for example false detections caused by radar shadowing or smooth impervious surfaces. 

To assess the generalisation of the proposed framework across diverse regions and sensor conditions, we trained and evaluated our model using a comprehensive dataset compiled from publicly available benchmarks, including Kuro Siwo and WorldFloods. Our framework not only establishes a new benchmark for all-weather flood monitoring but also demonstrates the critical role of remote sensing foundation models in overcoming the limitations of traditional, data-hungry fusion approaches.

How to cite: Chen, Y. C. and Wang, L. P.: Integrating SAR and Multispectral Satellite Observations for Flood Inundation Mapping: A Cross-Modal Fusion Framework Leveraging Foundation Models and Gated Attention Mechanism, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13502, https://doi.org/10.5194/egusphere-egu26-13502, 2026.

EGU26-13888 | ECS | Posters on site | HS6.5

A Comparative Assessment of Threshold-Based and Machine Learning Methods for Flood Detection 

Jawad Mones, Saeed Mhanna, Landon Halloran, and Philip Brunner

 

Flood mapping plays a key role in understanding hazard impacts, supporting emergency response, and guiding long-term risk planning. Remote sensing is now widely used in flood studies because it offers low-cost data, avoids the need for dangerous field surveys, and provides rapid observations over large areas. Despite these advantages, comparative research remains limited, particularly with respect to differences among flood-mapping algorithms, such as machine-learning versus threshold-based approaches, and the performance of optical versus radar sensors. This research addresses these gaps by applying multiple flood-mapping methods to the same flood event in Pakistan, and then comparing their performance with respect to a validation benchmark to provide a clearer insight into how data selection and methodological design influence flood detection outcomes

This study evaluates four distinct methods for mapping floods using multi-sensor satellite data. To ensure a fair comparison, three unsupervised machine-learning approaches including a synergetic Sentinel-1 and Sentinel-2 workflow, a method integrating harmonized Landsat–Sentinel data with radar, and a daily MODIS imagery technique were tested alongside a traditional Otsu thresholding baseline. All four were tested on the same 2025 Pakistan flood event, characterized by intense monsoon rains and flash flooding across regions such as Sindh and Punjab in mid- to late-2025.  The flood maps were then validated against UNOSAT flood reports for this event, where UNOSAT’s flood extent closely matches the results produced by the Sentinel-1/Sentinel-2 workflow, which yields the most conservative flood extent among the tested methods.

 Larger flood extents from some methods, especially the Sentinel-1 Otsu thresholding approach, include areas not clearly flooded in optical images. This happens because SAR backscatter also responds to wet soil and saturated vegetation, which a simple threshold can misclassify as water, leading to flood overestimation.

Overall, the results show that flood maps are not just different versions of the same answer, they reflect different satellite data and the utilized algorithms detect flooding. Approaches that combine multiple data sources with machine-learning strike a better balance, producing flood extents that are both spatially consistent and physically realistic. This indicates that multi-sensor, machine-learning–based methods are better suited for operational flood monitoring than simple thresholding, which is too sensitive to surface noise and often overestimates flooding. 

How to cite: Mones, J., Mhanna, S., Halloran, L., and Brunner, P.: A Comparative Assessment of Threshold-Based and Machine Learning Methods for Flood Detection, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13888, https://doi.org/10.5194/egusphere-egu26-13888, 2026.

EGU26-16468 | ECS | Orals | HS6.5

Multidecadal Changes and Trends in Global River Positions 

Elad Dente, John Gardner, Theodore Langhorst, and Xiao Yang

Rivers play a central role in shaping the Earth's surface and ecosystems through physical, chemical, and biological interactions. The intensity and locations of these interactions change as rivers continuously migrate across the landscape. In recent decades, human activity and climate change have altered river hydrology and sediment fluxes, leading to changes in river position, or migration. However, a comprehensive perspective on and understanding of these recent changes in the rate of river position shifts is lacking. To address this knowledge gap, we created a continuous global dataset of yearly river positions and migration rates over the past four decades and analyzed trends. The global annual river positions were detected using Landsat-derived surface water datasets and processed in Google Earth Engine, a cloud-based parallel computation platform. The resulting river extents and centerlines reflect the yearly permanent position, corresponding to the rivers’ location during base flow. This approach improves the representation of position changes derived from geomorphological rather than hydrological processes. To robustly analyze river position changes across different patterns and complexities and at large scales, we developed and applied a global reach-based quantification method.

Results show that while alluvial rivers maintain stable positions in certain regions, others exhibit trends in the rates of position change. For instance, the Amazon Basin, which has experienced significant deforestation and hydrological modifications, has shown increased rates of river position change in recent decades, directly modifying active floodplains. In this presentation, we will discuss the advantages, limitations, and applications of the global yearly river position dataset, offer insights into the changing rates of river position, and highlight current and future impacts on one of Earth’s most vulnerable hydrologic systems.

How to cite: Dente, E., Gardner, J., Langhorst, T., and Yang, X.: Multidecadal Changes and Trends in Global River Positions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16468, https://doi.org/10.5194/egusphere-egu26-16468, 2026.

Satellite-based surface water monitoring is essential for traking the spatiotemporal dynamics of global water bodies. However, most existing systems rely on a single mission or sensor modality, constraining both accuracy and temporal coverage. To overcome these limitations, we propose a multi-mission data fusion framework that integrates SAR Sentinel-1 and optical Sentinel-2 observations. Two U-Net convolutional neural networks were trained independently on the S1S2-Water dataset: one using Sentinel-1 sigma-nought backscatter (VV/VH) and the other using Sentinel-2 RGB and NIR bands, with terrain slope incorporated as ancillary input in both models. Predictive uncertainty is quantified via Monte Carlo dropout embedded within the networks, modeling pixel-wise predictions as Gaussian distributions. These probabilistic outputs are subsequently fused using a Bayesian framework and refined through sensor-specific exclusion masks. Evaluation across 16 geographically diverse test sites demonstrates that the fused probabilistic predictions achieve an overall IoU of 89%, highlighting the synergistic benefits of uncertainty-aware, multi-sensor integration. Furthermore, we show that model evaluation restricted to cloud-free optical imagery introduces substantial bias, limiting applicability for near-real-time monitoring. The proposed framework improves temporal availability, robustness, and reliability, advancing multi-satellite approaches for global surface water monitoring.

How to cite: Hassaan, M., Festa, D., and Wagner, W.: SAR and optical imagery for dynamic global surface water monitoring: addressing sensor-specific uncertainty for data fusion, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17524, https://doi.org/10.5194/egusphere-egu26-17524, 2026.

EGU26-18308 | Orals | HS6.5

RESCUE_SAT project: Leveraging Satellite Data to Improve Large‑Scale Flood Modeling 

Elena Volpi, Stefano Cipollini, Luciano Pavesi, Valerio Gagliardi, Richard Mwangi, Giorgia Sanvitale, Irene Pomarico, Aldo Fiori, Deodato Tapete, Maria Virelli, Alessandro Ursi, and Andrea Benedetto

The RESCUE_SAT project was launched as part of the “Innovation for Downstream Preparation for Science” (I4DP_SCIENCE) programme (Agreement no. 2025‑2‑HB.0), funded by the Italian Space Agency (ASI), with the goal of enhancing the performance of the RESCUE model through the integration of satellite data. RESCUE is a large‑scale inundation model that enables probabilistic flood‑hazard assessment over large areas by preserving computational efficiency while explicitly representing hydrologic-hydraulic processes along the full drainage network. Primarily based on digital terrain models (DTMs), RESCUE is a hybrid framework that combines a geomorphology-based representation of the river network with simplified hydrological and hydraulic formulations to estimate water levels and inundation extents. The central challenge of the RESCUE_SAT project is to deliver a flood‑modelling tool capable of providing a more reliable and detailed representation of both large‑scale hydrological behavior and local hydraulic processes, including flow interactions with structures such as levees, bridges and dams which are currently not explicitly represented in RESCUE. To this purpose, the Synthetic Aperture Radar (SAR) imagery acquired by the ASI’s COSMO-SkyMed constellation is processed using interferometric techniques to derive high-resolution digital elevation models (DEMs), reaching meter-scale resolution. Starting from high-resolution DEMs derived from COSMO-SkyMed satellite imagery, RESCUE_SAT enables the identification of the locations of structures that interacts with flow propagation, supporting their systematic mapping. Once the infrastructures have been identified and parameterized from the high-resolution DEM, the DEM is resampled and processed to a computationally advantageous coarser resolution, while the detected infrastructure elements are directly integrated into the hydrological–hydraulic model.

How to cite: Volpi, E., Cipollini, S., Pavesi, L., Gagliardi, V., Mwangi, R., Sanvitale, G., Pomarico, I., Fiori, A., Tapete, D., Virelli, M., Ursi, A., and Benedetto, A.: RESCUE_SAT project: Leveraging Satellite Data to Improve Large‑Scale Flood Modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18308, https://doi.org/10.5194/egusphere-egu26-18308, 2026.

EGU26-18518 | Orals | HS6.5

Automated Detection of Flood Events from CYGNSS: Observing Flood Evolution Along Propagating Tropical Waves  

Zofia Bałdysz, Dariusz B. Baranowski, Piotr J. Flatau, Maria K. Flatau, and Clara Chew

Flooding is a major natural hazard across the global tropics. Although flood occurrence is shaped by rainfall characteristics—including duration, frequency, and intensity—accurate prediction remains challenging. A key limitation is the lack of reliable, long-term flood databases that capture events across all spatial scales and durations, hindering a clear understanding of how rainfall variability translates into flood onset. This limitation is particularly critical in the Maritime Continent, where extreme rainfall is common and many small, short-lived, yet severe, floods remain undocumented. To address this limitation, we investigate whether a relatively new approach, global navigation satellite system reflectometry (GNSS-R), can help close this observational gap.

In this work, we assess whether data from the CYGNSS small-satellite constellation can be used to identify small- to regional-scale floods, including short-lived events. Our study focuses on Sumatra, an island within the Maritime Continent that is frequently affected by such hazards. A joint analysis of CYGNSS inundation estimates and two independent flood databases allowed us to evaluate how CYGNSS measurements can be used for flood detection. Three detailed case studies demonstrate that CYGNSS provides an unprecedented ability to monitor day-to-day changes in surface water extent, including floods at the urban scale. Specifically, we show that CYGNSS-derived inundation anomalies can clearly capture evolution of a flooding event, with the largest signature one day after known flood initiation. A systematic analysis of 555 flood events over a 21-month period enabled us to identify characteristic patterns in inundation anomalies that reliably distinguish flood events from non-flooding conditions, through the definition of an inundation-anomaly threshold and a maximum distance between CYGNSS detections and reported flood locations. We established that CYGNSS observations within 15 km not-only significantly differ from base-line conditions, but they allow tracking day-to-day flood dynamics as well.

The proposed methodology is transferable and can be applied to establish flood-inundation thresholds for any region within the global tropics, enabling automated detection of previously unreported flood events or the study of relationships between extreme precipitation and flood evolution. An example of its application is the automatic detection of flooding from CYGNSS data associated with subseasonal variability in tropical circulation: the passage of multiple convectively coupled Kelvin waves embedded within an active Madden–Julian Oscillation in July 2021. These waves propagated eastward across the Maritime Continent, triggering extreme rainfall and widespread flooding in equatorial Indonesia and East Malaysia. The day-to-day evolution of floods could be observed alongside the propagating waves, with the termination of the MJO coinciding with the cessation of the flood events.

Relying on low-cost small satellites, this approach shows strong potential for future scalability with larger constellations, ultimately improving flood monitoring and advancing our understanding of how rainfall patterns shape flood dynamics across global tropics.

How to cite: Bałdysz, Z., Baranowski, D. B., Flatau, P. J., Flatau, M. K., and Chew, C.: Automated Detection of Flood Events from CYGNSS: Observing Flood Evolution Along Propagating Tropical Waves , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18518, https://doi.org/10.5194/egusphere-egu26-18518, 2026.

Accurate long-term monitoring of surface water dynamics in the Niger River and Lake Chad basins is crucial for regional ecological security and sustainable water resource management. However, such monitoring is often hindered by insufficient continuous high-frequency observations—necessary to capture rapid shifts between permanent and seasonal water bodies in semi-arid transition zones—as well as by persistent cloud cover. To address these limitations, we developed a spatio-temporal data fusion framework designed to delineate detailed evolutionary patterns and regime shifts in surface water. Our methodology integrates Sentinel-1 SAR, Sentinel-2 optical imagery, and digital elevation model (DEM) data, adopting a “zoning modeling” strategy to reduce sensor-specific biases and environmental noise, thereby producing annual and seasonal surface water distribution maps. Furthermore, we developed a pixel-level, climate-coupled model based on inundation frequency to quantify changes in the extent, timing, and type of water bodies across a multi-year time series. Integration of these outputs elucidated the spatial heterogeneity of water resources throughout the study region from 2015 to 2024. Validation using randomly distributed reference samples demonstrated strong consistency, with overall accuracy exceeding 90%, confirming the robustness of our framework. Through an ecology-oriented classification scheme, we identified permanent water bodies—largely concentrated in the southern reaches of the Niger River main channel and the central zone of Lake Chad—as serving a “core support” function within the ecosystem. In contrast, seasonal water bodies followed a “dense in the south, sparse in the north” spatial pattern and acted as critical “ecological buffers” for arid northern areas. Notably, seasonal water extent expanded significantly during high-rainfall years such as 2018 and 2022, underscoring its pronounced sensitivity to climatic variability. Compared with current state-of-the-art approaches, the proposed framework enables characterization of high-frequency surface water dynamics and associated ecological interactions as continuous spatio-temporal fields, thereby providing a reliable and scalable tool to inform sustainable watershed management strategies across Africa.

How to cite: Du, L., You, S., Ye, F., and He, Y.: Tracking Dynamic Regimes and Ecological Functions of Surface Water in the Niger-Lake Chad Basins through Multi-Source Fusion (2015–2024), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19055, https://doi.org/10.5194/egusphere-egu26-19055, 2026.

EGU26-19963 | ECS | Orals | HS6.5

Development of routine flood mapping using SAR satellite observation for long-term monitoring system in the flood-prone regions, Cambodia 

Chhenglang Heng, Vannak Ann, Thibault Catry, Vincent Herbreteau, Cyprien Alexandre, and Renaud Hostache

Monitoring inland surface water in near-real time is a key challenge in cloud-prone tropical regions.  Recently, Synthetic Aperture Radar (SAR) products have been widely used to detect surface water. Our area of interest, the Tonle Sap Lake region is a complex environment where very large areas and floodplains are partially or fully submerged seasonally. As the population living around the lake strongly rely on the seasonal flooding dynamics for their socio-economic activities and can at the same time be at risk due to extreme flooding events, it is of main importance to develop tools for the monitoring of flooded areas. In this context, we are adopting and evaluating an algorithm which relies on parametric thresholding, and region growing approaches applied over time series of Sentinel-1 (S1) SAR backscatter images (VV and VH). To evaluate the produced water extent maps based on VV and VH polarizations, we used a cross evaluation using multi-sensor products: high-resolution optical data such as Sentinel-2 (S2) and the coarser resolution Sakamoto flood extend derived from MODIS product. The comparison is made using the Critical Success Index (CSI) and Kappa coefficient performance metrics. During the dry season, the VV polarization demonstrated very good performance using S2-derived maps as a reference, with CSI of 0.84 and a Kappa coefficient of 0.91, indicating highly accurate surface water detection. Performance was similar using the Sakamoto product as a reference (CSI=0.87). However, performance dropped during the rainy season, with the VV polarization's CSI decreasing to 0.76 comparing S2, reflecting challenges in detecting water in the extensive flooded vegetation areas. VH polarization consistently overestimated water extent by misclassifying wet vegetation and rice fields. A merge of VV and VH product yielded an intermediate performance, improving water detection in vegetated areas compared to VV alone. This comprehensive, multi-sensor and multi-season assessment clarifies the specific strengths of each S1 polarization, showing VV's superiority for open water mapping, especially in the dry season. It underscores the importance of selecting the appropriate product (VV for open water, merged for total inundation) and considering seasonal context for operational monitoring, thereby demonstrating the algorithm's robustness while also defining its operational limitations.

How to cite: Heng, C., Ann, V., Catry, T., Herbreteau, V., Alexandre, C., and Hostache, R.: Development of routine flood mapping using SAR satellite observation for long-term monitoring system in the flood-prone regions, Cambodia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19963, https://doi.org/10.5194/egusphere-egu26-19963, 2026.

The research focused on developing the framework for assessing marine, nearshore and transitional waters across Ireland and validated for generalization of the framework across at any geospatial scale using remote sensing (RS) products. To the best of authors knowledge, existing most of the studies only have demonstrated for retrieving particular water quality (WQ) indicators like turbidity, salinity or chlorophyll a without in depth validation results. Recently the authors comprehensively reviewed several studies focusing on the RS applications for assessing WQ using computational intelligence techniques (CIT) like machine learning, artificial intelligence, statistical approaches etc. Unfortunately, the reviewed findings reveals that most of the research are questionable in terms of using data transparency, and validation with independent or other geospatial domains applications of the existing developed tools. Therefore, the research aim was to develop a novel framework and validated with independent datasets including new domain(s) adaptation or validation. For developing the framework, to achieve the goal of the research, the study utilized Sentinel-3 (S3) OLCI RS reflectance data. For obtaining RS data, the study utilized S3-OLCI level 3(L3) and level 4 (L4) reflectance data Rhow_1 to Rhow_11 form the Copernicus Marine Services (CMS) repository datasets for 2016 to 2024. To obtain the overall WQ, the research considered 49 (in-situ) EPA, Ireland monitoring sites across various transitional and coastal waterbodies for computing the overall WQ (IEWQI scores) scores using recently developed and widely validated the IEWQI model. After than the RS data prepared and match-up with 49 considering monitoring sites. For predicting IEWQI scores, the research utilized the multi-scale signal processing framework (MSSPF) by following configurations: data augmentations: 2x to 20x, noise level from 0.0001 to 0.05, and data spilled ratios 60-20-20 and 70-20-10, respectively for train, test and validation of 43 CIT models using RS data from 2016 to 2023 both L3 and L4, whereas the 2024 dataset using for testing independent dataset to generalize the model prediction capabilities. Utilizing four identical model performance evaluation metrics, the results reveals that the PyTorchMLP could be effective (train performance : R2 = 0.86, RMSE =0.09, MSE = 0.008, and MAE = 0.067; test performance : R2 = 0.84, RMSE =0.094, MSE = 0.008, and MAE = 0.071; and validation performance : R2 = 0.81, RMSE =0.095, MSE = 0.009, and MAE = 0.074, respectively at 7x augmentation with 0.0001 of noise level for 60-20-20) compared to the 43 CIT models in terms of predicting and validating independent dataset (independent dataset validation performance for 2024 : R2 = 0.62, RMSE =0.164, MSE = 0.026, and MAE = 0.12). Based on the predicted IEWQI scores, the WQ ranked “marginal”, “fair” and “good” categories for Irish waterbodies. The findings of the framework align with the traditional EPA, Ireland monitoring approaches. However, findings of the research reveals that the proposed framework could be effective to monitoring WQ general purposes using RS data across any geospatial resolution.

Keywords: remote sensing; Copernicus database; MSSPF, IEWQI, Ireland.

How to cite: Uddin, M. G., Diganta, M. T. M., Sajib, A. M., Rahman, A., and Indiana, O.: A comprehensive framework for assessing marine, nearshore and transitional waters quality integrating Irish Water quality Index (IEWQI) model from remote sensing products using computational intelligence techniques, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20016, https://doi.org/10.5194/egusphere-egu26-20016, 2026.

EGU26-20097 | ECS | Orals | HS6.5

Comprehensive validation of the benefits of multi-sensor flood monitoring 

Chloe Campo, Paolo Tamagnone, Guy Schumann, Trinh Duc Tran, Suelynn Choy, and Yuriy Kuleshov

Multi-sensor methodologies are gaining traction within flood monitoring research, grounded in the rationale that data fusion from diverse sources mitigates uncertainty and improves spatiotemporal coverage. However, these assumed benefits are rarely quantified.

This work aims to comprehensively compare the performances of multi-sensor and single-sensor approaches to understand to what extent increasing the number and variegate data source may improve the detection rate and temporal characterisation of flood events. A multi-sensor flood monitoring approach using AMSR2 and VIIRS data is assessed against each sensor individually and against standard benchmarks in EO-based flood detection (e.g., MODIS and Sentinel-1)  for major flood events in the Savannakhet Province of Laos.

The comparative analysis evaluates multiple metrics. First, detection comparison classifies events as captured by each considered approach, multi-sensor only, each individual sensor only, or missed by all, to directly quantify the improvement attributable to multi-sensor integration. The spatial agreement is assessed between the multi-sensor and single sensor approaches for jointly detected flood events. Additionally, the temporal component is characterized by an examination of the observation frequency, maximum observation gaps, and peak capture timing. Lastly, the various detection outcomes are related to event characteristics, including cloud cover persistence, flood magnitude, duration, and flood type, quantifying the conditions under which a multi-sensor approach performs optimally.

How to cite: Campo, C., Tamagnone, P., Schumann, G., Duc Tran, T., Choy, S., and Kuleshov, Y.: Comprehensive validation of the benefits of multi-sensor flood monitoring, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20097, https://doi.org/10.5194/egusphere-egu26-20097, 2026.

Integrated Monitoring of Lake Garda with Radar, Optical Sensors and In Situ Instruments: Insights from the SARLAKES Project

Virginia Zamparelli1, Simona Verde1, Andrea Petrossi1, Gianfranco Fornaro1, Marina Amadori2,3, Mariano Bresciani2, Giacomo De Carolis2, Francesca De Santi4, Matteo De Vincenzi3, Giulio Dolcetti3, Ali Farrokhi3, Raffaella Frank2, Nicola Ghirardi2,5, Claudia Giardino2, Fulvio Gentilin6, Alessandro Oggioni2, Marco Papetti6, Gianluca Pari7 Andrea Pellegrino2, Sebastiano Piccolroaz3, Tazio Strozzi8, Marco Toffolon3, Maria Virelli7, Nestor Yague-Martinez9, and Giulia Valerio6

 

1Institute for Electromagnetic Sensing of the Environment (IREA), National Research Council, Naples, Italy

2Institute for Electromagnetic Sensing of the Environment (IREA), National Research Council, Milan, Italy

3Department of Civil, Environmental and Mechanical Engineering (DICAM), University of Trento, Trento, Italy

4Institute for Applied Mathematics and Information Technologies (IMATI), National Research Council, Milan, Italy

5 Institute for BioEconomy (IBE), National Research Council, Sesto Fiorentino, Italy

6Department of Civil, Environmental, Architectural Engineering and Mathematics (DICATAM), University of Brescia, Brescia, Italy

7Italian Space Agency (ASI), Rome, Italy

8GAMMA Remote Sensing, Gümligen, Switzerland

9Capella Space Corp., San Francisco, CA, USA

 

SARLAKES (SpatiAlly Resolved veLocity and wAves from SAR images in laKES) is a PRIN (Projects of National Interest) project funded in 2022 by the Italian Ministry of University and Research. The project is now in its final phase and is scheduled to end at the beginning of 2026. The project developed a novel, advanced and adaptable tool capable of accurately measuring water dynamics in medium- and large-sized lakes.

A key and innovative aspect of the project is the use of spaceborne Synthetic Aperture Radar (SAR) data, which are widely exploited for routine observation of the marine environments but remain relatively underutilized for lake monitoring. SARLAKES investigated the capability of SAR imagery to retrieve the spatial distribution of wind fields, surface currents, and wind-generated waves in lacustrine environments.

The project considers Lake Garda and Lake Geneva as case studies, with Lake Garda—the largest lake in Italy—selected as the primary test site due to the research group’s long-standing experience and the availability of extensive historical data.

This contribution presents the main results obtained over two years of project activity, with particular emphasis on outcomes from a multidisciplinary field campaign conducted on April 2025. The campaign aimed to reconstruct lake surface currents during a strong wind event in the peri-Alpine Lake Garda region.

The field instrumentation included a wave buoy, an acoustic Doppler current profiler (ADCP), Lagrangian drifters, anemometers, a ground-based radar, fixed cameras, a drone, and a conductivity–temperature–depth profiler. Satellite acquisitions from the COSMO-SkyMed Second Generation and Capella Space SAR sensors, as well as from the optical sensor PRISMA were scheduled over the study area during the campaign. Archive data from Sentinel-1, Sentinel-2, Sentinel-3, Landsat, and COSMO-SkyMed missions were also utilized.

The project demonstrates how the integration of in-situ instrumentation, spatially distributed flow measurements from remote sensing, and hydrodynamic modeling provides a comprehensive and scalable approach to next-generation monitoring of complex lake systems.

How to cite: Zamparelli, V. and the SARLAKES project team: Integrated Monitoring of Lake Garda with Radar, Optical Sensors and In Situ Instruments: Insights from the SARLAKES Project, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21000, https://doi.org/10.5194/egusphere-egu26-21000, 2026.

Semi-urban vegetation systems play a critical role in ecosystem stability but are increasingly exposed to flood hazards due to climate variability and rapid land-use change. Accurate flood detection in such system remains challenging because radar backscatter is influenced by complex and mixed scattering mechanisms arising from vegetation, built-up structures, and surface water. Conventional intensity-based flood indices struggle to separate flooded vegetation from non-flooded rough surfaces and tend to miss inundated areas under mixed land-cover conditions. To address these limitations, this study presents a physically interpretable flood detection framework that integrates Synthetic Aperture Radar polarimetric descriptors with a machine learning classifier. The proposed approach utilizes dual-polarized Sentinel-1 SAR data to derive polarimetric features from Stokes parameters and the covariance matrix. Specifically, the Degree of Polarization and Linear Polarization Ratio are combined with eigenvalue-based information to capture changes in both amplitude and polarization state between pre-flood and during-flood conditions. These descriptors are integrated into a novel Flood Index (FI) designed to distinguish flooded urban areas dominated by double-bounce scattering from flooded vegetation characterized by depolarized volume scattering. Unlike commonly used indices such as the Normalized Difference Flood Index (NDFI) or VH/VV ratio, the proposed FI exploits polarization behaviour rather than relying solely on backscatter intensity. A Random Forest classifier is trained on the proposed FI using a tile-based sampling strategy to handle class imbalance between flooded and non-flooded pixels. The framework is evaluated across three flood events representing diverse geographic and land-cover conditions: the 2019 Typhoon Hagibis flood in Japan, the 2023 Yamuna River flood in India, and the 2023 Larissa flood in Greece. Model performance is assessed using multiple accuracy metrics, including F1 score, Intersection over Union (IoU), False Positive Rate (FPR), and False Negative Rate (FNR). Results demonstrate that the Random Forest model trained on the proposed Flood Index consistently outperforms threshold-based Otsu methods and NDFI across all study areas. The approach achieves F1 scores ranging from 0.81 to 0.86 and IoU values between 0.70 and 0.76, while maintaining a relatively low False Negative Rate (0.09-0.17), that is critical for minimizing missed flooded areas in disaster response applications. Sensitivity and ablation analyses further confirm the robustness of the Flood Index to speckle noise and highlight the complementary contribution of its individual components. Overall, the proposed framework offers a transferable and computationally efficient solution for flood mapping in semi-urban vegetation systems using widely available dual-polarized SAR data. The results highlight its potential for scalable flood monitoring and rapid damage assessment across regions with heterogeneous land-cover conditions.

How to cite: Adhikari, R. and Bhardwaj, A.: SAR polarimetry-based machine learning method for flood detection in semi-urban vegetation systems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21063, https://doi.org/10.5194/egusphere-egu26-21063, 2026.

EGU26-21507 | ECS | Posters on site | HS6.5

Flood Susceptibility Mapping with GFI 2.0 and Artificial Intelligence Models 

Jorge Saavedra Navarro, Ruodan Zhuang, Caterina Samela, and Salvatore Manfreda

Floods are among the most damaging natural hazards, motivating the development of rapid and scalable tools for floodplain mapping across multiple return periods and for post-event assessment. The Geomorphic Flood Index (GFI) is widely used to identify flood-prone areas using topographic information, but it can exhibit reduced reliability under complex hydraulic conditions—particularly near confluences where backwater controls water levels—and it may systematically overestimate inundation extents when used as a binary classifier.

This study advances the GFI framework by explicitly accounting for backwater effects at river confluences and along tributary junctions. In parallel, to reduce the intrinsic overestimation of GFI-derived floodplains, we test a suite of Artificial Intelligence (AI) classifiers—Random Forest, XGBoost, and Neural Networks—trained through a multi-parametric formulation that combines GFI with auxiliary predictors, including precipitation, lithology, land use, and slope. The approach is evaluated across multiple Italian catchments, using satellite-derived inundation and hydrodynamic simulations as independent benchmarks. Model performance is quantified against the baseline GFI approach using a standard threshold-based binary classification using an optimal cutoff.

The proposed framework aims to improve post-event flood delineation under observational constraints (e.g., satellite data gaps due to cloud cover, vegetation, or imaging limitations) and to provide a computationally efficient surrogate for extending hydrodynamic information to additional return periods or large basins where full numerical modelling is impractical. Preliminary results indicate that Random Forest provides the most robust performance across study sites. Incorporating backwater effects yields clear gains at confluences, primarily by reducing omission errors and improving the representation of hydraulically controlled inundation patterns. Moreover, the AI-based correction substantially mitigates the overestimation typically associated with standard GFI mapping, resulting in floodplain delineations that are more consistent with complex hydrodynamic processes and suitable for scalable flood hazard applications.

How to cite: Saavedra Navarro, J., Zhuang, R., Samela, C., and Manfreda, S.: Flood Susceptibility Mapping with GFI 2.0 and Artificial Intelligence Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21507, https://doi.org/10.5194/egusphere-egu26-21507, 2026.

EGU26-21622 | ECS | Orals | HS6.5

Mapping and modeling coastal flood dynamics using remote sensing and hydrodynamic models 

Giovanni Fasciglione, Guido Benassai, Gaia Mattei, and Pietro Patrizio Ciro Aucelli

This study presents an integrated and multidisciplinary methodology for investigating coastal flooding and morphodynamic processes in low-lying coastal environments, with a comparative application to two geomorphologically distinct Mediterranean coastal plains: the Volturno Plain and the Fondi Plain. The methodological framework combines high-resolution topographic and bathymetric datasets, aerial remote sensing, sedimentological analyses, statistical wave climate assessment, numerical hydrodynamic modelling, and relative sea-level rise scenarios that incorporate both eustatic trends and local vertical land movements. This approach enables a robust evaluation of how differing coastal configurations influence flooding susceptibility under extreme marine conditions.

For both study areas, the topographic baseline was derived from 2 m resolution LiDAR-based Digital Terrain Models, subsequently refined using site-specific datasets. In the Volturno Plain, extensive GNSS field surveys were conducted along the beach between Volturno and Regi Lagni river mouths. In the Fondi Plain, DTM refinement relied on aerial drone surveys carried out over the beach sector between the Canneto and Sant’Anastasia river mouths. Photogrammetric processing of aerial imagery allowed the generation of high-resolution surface models, which were integrated with the existing LiDAR DTM to enhance the depiction of subtle morphological features critical for flood propagation.

Sedimentological characterization was performed to constrain morphodynamic responses. Granulometric samples were collected along cross-shore transects at elevations ranging from −1.5 m to +2 m. Grain-size distribution analyses supported the calibration and interpretation of sediment transport and wave dissipation processes within numerical models.

Bathymetric modelling was based on high-precision single-beam echo-sounder surveys, with depth data corrected for tidal variations using official tide-gauge records. Emerged and submerged datasets were merged into continuous topo-bathymetric models, ensuring consistency in vertical reference systems and numerical stability.

Marine storms were identified through the analysis of offshore buoy records using a Peak Over Threshold approach. Storm events were classified into five classes using their Storm Power Index calculated by combining significant wave height and event duration. Representative events were selected as boundary conditions for coupled hydrodynamic simulations performed with Delft3D and XBeach. Simulations were run for future scenarios based on high-emission IPCC projections (SSP 5-8.5), integrating local sea-level rise, local subsidence rates, and highest tidal and surge levels.

A comparative analysis of the simulation outcomes highlights marked differences between the two coastal plains. The Volturno Plain results highly prone to inundation, with storm surges overtopping dune systems and propagating inland due to low elevations, local subsidence, and limited effectiveness of existing coastal defenses. Conversely, the Fondi Plain exhibits significantly reduced flood penetration. The presence of a wide bar system, coupled with efficient coastal defense structures, promotes substantial dissipation of incoming wave energy. As a result, even under intense storm conditions, inundation remains confined to a narrow coastal strip immediately landward of the beach.

Overall, the comparative methodological application demonstrates how coastal morphology, sedimentological properties, and defense systems critically control flood dynamics. The proposed framework provides a transferable and decision-oriented tool for assessing coastal vulnerability and supporting adaptation strategies in heterogeneous low-lying coastal settings under climate change pressure.

How to cite: Fasciglione, G., Benassai, G., Mattei, G., and Aucelli, P. P. C.: Mapping and modeling coastal flood dynamics using remote sensing and hydrodynamic models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21622, https://doi.org/10.5194/egusphere-egu26-21622, 2026.

EGU26-21631 | ECS | Posters on site | HS6.5

Assessment of Multi-Mission Satellite Altimetry GDR L2 Products for River Water Surface Elevation in the Ganga Basin 

Barun Kumar, Shyam Bihari Dwivedi, and Shishir Gaur

Precise monitoring of water surface elevation (WSE) in data-deficient areas such as the Ganga River stretch is essential for hydrological modelling, flood prediction, and comprehensive water resource management. This study introduces a comprehensive evaluation framework for Level-2 Geophysical Data Records (GDR L2) derived from various satellite altimetry missions, including Sentinel-3A/B, Sentinel-6A, Jason-3, and SWOT Nadir, validated against in-situ gauge stations from the Central Water Commission (CWC) across a range of hydrological conditions. The process includes advanced geographical analysis. Gaussian-process Kriging interpolation generates continuous longitudinal WSE profiles across strategically placed virtual stations; rigorous outlier detection employs interquartile range (IQR) and Hampel filters; bias correction employs dry-season median alignment to a common orthometric datum; and Kalman filter smoothing effectively reduces measurement noise while preserving critical hydrological signal dynamics.

Comprehensive performance evaluations employ co-located time series analysis, scatter plots, and flow duration curves (FDCs), with seasonal stratification distinguishing monsoon high-flow variability from stable non-monsoon baseflow conditions. The evaluation stresses physically significant parameters based on Kling-Gupta Efficiency (KGE) and RMSE. Sentinel-6A is the strongest performer in all situations with high non-monsoon accuracy (KGE 0.894, RMSE 0.089 m) and monsoon performance (KGE 0.57, RMSE 3.08 m) despite turbulent flow issues, but SWOT Nadir's processing potential is limited by specific hooking artifacts. During non-monsoon periods, measurement reliability is consistently 2-4 times higher. This proven multi-mission system demonstrates satellite altimetry as an operationally viable method for WSE retrieval in major braided rivers, allowing for accurate rating curve generation and discharge computation. In future machine learning data fusion and hydrodynamic modelling can be incorporated to increase basin-scale forecast capabilities.

How to cite: Kumar, B., Dwivedi, S. B., and Gaur, S.: Assessment of Multi-Mission Satellite Altimetry GDR L2 Products for River Water Surface Elevation in the Ganga Basin, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21631, https://doi.org/10.5194/egusphere-egu26-21631, 2026.

EGU26-21734 | Posters on site | HS6.5

Evaluating Copernicus Global Flood Monitoring (GFM) Service trade-offs in near-real-time flood mapping 

Shagun Garg, Ningxin He, Sivasakthy Selvakumaran, and Edoardo Borgomeo

Near-real-time satellite-based flood maps support disaster risk management and emergency response. One widely used service is the Global Flood Monitoring (GFM) product of the Copernicus Emergency Management Service, launched in 2021 and based on Sentinel-1 Synthetic Aperture Radar (SAR) data. The GFM service combines three flood-mapping algorithms: pixel-based thresholding, region-based approaches, and change-detection techniques, merged using a majority-voting scheme to generate the final flood extent product. Another key strength of the GFM service is its rapid analysis, providing flood maps within approximately five hours of satellite image acquisition through a fully automated processing chain. As the product is increasingly relied upon by practitioners and decision-makers, there is a growing need to assess its accuracy and robustness. Understanding false alarms and missed detections is critical for improving the reliability and usability of the service.


In this study, we systematically compare GFM flood maps across twenty real-world flood events using high-resolution reference datasets. To ensure temporal consistency, the GFM-derived flood maps are generated using Sentinel-1 acquisitions from the same day as the reference observations. Spatial agreement between datasets is quantified using the Intersection-over-Union metric.


Our results suggest that the GFM service performs well for large, extensive flood events but degrades for smaller, localized ones. Many of the observed errors come not from flood detection itself, but from inaccuracies in the reference water layer - while surface water is correctly identified, misclassification of permanent or seasonal water bodies leads to false alarms and missed floods. We evaluate the three-underlying flood-mapping algorithms individually for consistent patterns of misdetection or false alarms. In addition, we develop an automated framework to rapidly compare any external flood map with the GFM outputs, enabling near-instant evaluation of agreement and error patterns. 


This framework provides practical insights into where and why the GFM services achieve successes and failures and offers continuous validation and iterative improvement of global flood mapping services. 

How to cite: Garg, S., He, N., Selvakumaran, S., and Borgomeo, E.: Evaluating Copernicus Global Flood Monitoring (GFM) Service trade-offs in near-real-time flood mapping, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21734, https://doi.org/10.5194/egusphere-egu26-21734, 2026.

EGU26-22077 | Orals | HS6.5

A fully automatic processing chain for the systematic monitoring of surface water using Copernicus Sentinel 1 satellite data: first results of the SCO-CASCADES project. 

Renaud Hostache, Cyprien Alexandre, Chhenglang Heng, Thibault Catry, Vincent Herbreteau, Vannak Ann, Christophe Révillion, and Carole Delenne

Water is essential to life and health of various ecological and social systems. Unfortunately, water is one of the natural resources most impacted by climate change, with increasingly intense hydro-meteorological extremes (floods, droughts, etc.) and growing societal demand. To help manage this vulnerable resource, it is vital to assess and monitor its availability on a regular basis, as well as to track its trajectory over time to better understand the impact of global change on it. Surface water (lakes, rivers, flood plains, etc.) represents an important component of total water resources, and it is of primary importance to monitor it to better understand and manage the consequences of climate change. Surface water resources provide populations around the world with essential ecosystem services such as power generation, irrigation, drinking water for humans and livestock, and space for farming and fishing.

In this context, the SCO-CASCADES project implements end-to-end processing chains for satellite Earth observation data, including Sentinel-1 and 2 (S-1 and S-2), in order to provide surface water products (surface water body and inundation depth maps) that will be made available via an interactive platform co-constructed with identified users.

In the first phase of the project a fully automated Sentinel-1 based processing chain has been implemented. This chain is based on automatic multiscale image histogram parameterization followed by thresholding, region growing and chain detection applied on individual, subsequent pairs, and time series of S1 images. This chain enables us to derive various products: i) an exclusion layer identifying areas where water cannot be detected on Sentinel 1 image (e.g. Urban and forested areas), ii) permanent seasonal water body maps, iii) a water body map for each S1 image, iv) an uncertainty map characterizing the water body classification uncertainty, v) an occurrence map providing the number of times (over the time series) each pixel was covered by open water.

Here, we propose to present and evaluate the robustness of the processing chain and the resulting maps produced using multi-year S1 time series over two large scale sites: the Mekong flood plains between Kratie, the Tonle Sap lake and the Mekong Delta, and the Tsiribihina basin in Madagascar. The kappa score obtained from the comparison between S1 and S2-derived maps shows a good agreement yielding CSI and Kappa Cohen scores most of the time higher than 0.7 and sometimes reaching values higher than 0.9.

How to cite: Hostache, R., Alexandre, C., Heng, C., Catry, T., Herbreteau, V., Ann, V., Révillion, C., and Delenne, C.: A fully automatic processing chain for the systematic monitoring of surface water using Copernicus Sentinel 1 satellite data: first results of the SCO-CASCADES project., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22077, https://doi.org/10.5194/egusphere-egu26-22077, 2026.

NP5 – Predictability

EGU26-153 | ECS | Orals | NP5.1

WeGen FastEvaluation: An open-source tool for the evaluation and comparison of machine learning models in weather and climate applications 

Ilaria Luise, Savvas Melidonis, Julius Polz, Sorcha Owens, Timothee Hunter, Christian Lessig, and Michael Tarnawa

The next generation of machine learning (ML) weather and climate models is increasingly trained on a wide variety of datasets, including reanalyses, forecasts and observations . This diversity can typically not be handled by existing evaluation tools that are often limited to gridded data or fixed lead times Furthermore, many existing evaluation frameworks are developed internally by institutions, remain closed-source, and lack interoperability across platforms and high-performance computing (HPC) environments. This creates a gap in the ability to systematically assess model skill across different data streams, experiments, and computing infrastructures.

The WeGen FastEvaluation tool, developed within the WeatherGenerator project, aims to bridge this gap. It provides a flexible, open-source framework designed to evaluate machine learning–based weather prediction models across a wide range of dataset types and formats. Unlike most existing tools, WeGen FastEvaluation makes minimal assumptions about data structure, allowing consistent analysis of both gridded and unstructured inputs, deterministic and probabilistic outputs, and multiple forecast lead times. Built on xarray, the WeGenFastEvaluation supports multi-dimensional data handling, including probabilistic outputs and ensemble forecasts. The tool enables efficient computation of skill metrics and generation of 2D visualizations, allowing users to compare an arbitrary number of model runs across different data streams and forecast configurations.

The presentation will introduce the design and capabilities of the WeGen FastEvaluation, highlighting its integration within the WeatherGenerator workflow. Through examples, we demonstrate how the WeGen FastEvaluation tool enables consistent benchmarking, collaborative analysis across HPC systems, and reproducible ML-for-weather research.



How to cite: Luise, I., Melidonis, S., Polz, J., Owens, S., Hunter, T., Lessig, C., and Tarnawa, M.: WeGen FastEvaluation: An open-source tool for the evaluation and comparison of machine learning models in weather and climate applications, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-153, https://doi.org/10.5194/egusphere-egu26-153, 2026.

EGU26-1553 | ECS | Orals | NP5.1

Deriving meaning from metrics – a new approach for machine learning nowcasting verification 

Jakub Lewandowski, Leif Denby, and Andrew Ross

Nowcasting - the prediction of weather conditions over the next few hours - is critical for mitigating the impacts of severe convective storms. Machine learning offers new opportunities for improving nowcasting, particularly for convective precipitation, where traditional numerical models struggle. Yet, despite rapid progress in model development, evaluating these models remains a major challenge. Current verification practices typically rely on a narrow set of standard metrics that often fail to capture the complexity of atmospheric phenomena and cannot distinguish between different types of errors, providing limited insight into the specific weaknesses of the models.

This research introduces a comprehensive verification framework that combines carefully crafted datasets with sensitivity analyses, aiming to transform metric-based evaluation into a more informative process. Synthetic datasets are generated using ArtPrecip, a novel tool that randomly generates radar-like precipitation fields while allowing full control over properties such as motion, initiation, and evolution. Observational radar data are classified based on synoptic setting and observed precipitation properties, using different dimension-reduction methods. Sensitivity analyses examine how existing metrics respond to various error patterns, providing guidance on interpreting benchmark results.

The resulting system provides a well-defined and well-described set of benchmarks and enables reproducible, objective, and meaningful comparison of models. By addressing gaps in evaluation methodology, this work contributes to a more robust assessment of machine learning nowcasting skill and its applicability to severe weather forecasting.

How to cite: Lewandowski, J., Denby, L., and Ross, A.: Deriving meaning from metrics – a new approach for machine learning nowcasting verification, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1553, https://doi.org/10.5194/egusphere-egu26-1553, 2026.

EGU26-1764 | ECS | Posters on site | NP5.1

Spectral representations for regional AI-based weather prediction 

Emily O'Riordan

Both dynamical and AI-based NWP have seen success in using spectral transformations to represent atmospheric variables efficiently. In particular, Fourier-based representations are widely adopted due to fast computational methods and compact encoding of large-scale structure. However, as the NWP community targets higher-resolution models, Fourier-bases may inadequately represent the sharp gradients and multi-scale features that often characterise extreme weather events. Furthermore, for limited-area domains, Fourier representations can impose artificial periodicity, making them less physically appropriate.

In this work, we investigate whether alternative spectral transformations better support AI-based NWP in regional, extreme-weather settings. We systematically compare neural forecasting models trained using Fourier, wavelet, and Legendre spectral representations, assessing their ability to predict multiple atmospheric variables over the Aotearoa New Zealand domain.  Wavelet and polynomial bases are explicitly designed for bounded domains and provide multi-scale, non-periodic representations, making these transformations more suitable for the regional forecasting task.

Aotearoa New Zealand provides an ideal test-bed for these methods, as a region with complex coastlines, steep orography, and frequent exposure to high-impact weather systems. Models are trained and evaluated on reanalysis datasets (ERA5 and BARRA-2), using standard verification metrics and case studies of major Aotearoa New Zealand storms such as Cyclones Gabrielle and Bola. Our results demonstrate that spectral choice has a measurable impact on forecast skill, particularly for extremes and fine-scale structure.

By analysing how different spectral representations influence AI-NWP performance in a regional context, this work provides guidance on the appropriate use of spectral methods for limited-area forecasting, and contributes to the development of more accurate and physically consistent AI-driven weather prediction systems for localised and extreme events.

How to cite: O'Riordan, E.: Spectral representations for regional AI-based weather prediction, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1764, https://doi.org/10.5194/egusphere-egu26-1764, 2026.

EGU26-2056 | ECS | Posters on site | NP5.1

An NWP-Free, Observation-Driven Deep Learning Approach to Heavy-Rainfall Nowcasting Beyond the Three-Hour Limit  

Ryu Shimabukuro, Tomohiko Tomita, Tsuyoshi Yamaura, and Ken-ichi Fukui

Quasi-stationary convective bands over Kyushu, Japan, frequently trigger rainy-season disasters, and hours with ≥50 mm h−1 rainfall are increasing. Yet skillful nowcasts beyond 3 h remain limited. This study presents FlowsNet, an observation-based multi-sensor fusion model that learns directly from radar/rain gauge-analyzed precipitation, surface variables from ground stations, geostationary satellite imagery, and satellite-derived precipitation context. The model targets category-4 (C4; ≥50 mm h−1) rainfall and incorporates two attention mechanisms: a channel-wise module that weights informative modalities and a spatial module that aligns features with banded structures at multi-hour leads. Training uses a tail-aware ordinal loss that couples focal reweighting with Earth Mover’s Distance to highlight rare extremes. FlowsNet maintains a non-zero C4 Critical Success Index through 6 h. From 4 to 6 h, it matches or exceeds the Japan Meteorological Agency’s very-short-range forecast, and it outperforms a leading extrapolation method and current deep-learning nowcasters. Case studies show preserved band geometry and corridor placement at long lead over complex terrain. Ablation experiments identify satellite water-vapor context and near-surface humidity as key for long-lead C4 prediction; combining satellite context with surface observations stabilizes placement and reduces false alarms. By avoiding numerical weather prediction model state and objective analyses/reanalyzes, the approach reduces latency and hardware demand, improves portability and resilience when model cycles degrade, and offers a practical route to earlier and more transferable warnings for extreme rainfall events.

How to cite: Shimabukuro, R., Tomita, T., Yamaura, T., and Fukui, K.: An NWP-Free, Observation-Driven Deep Learning Approach to Heavy-Rainfall Nowcasting Beyond the Three-Hour Limit , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2056, https://doi.org/10.5194/egusphere-egu26-2056, 2026.

Rapid population growth and the continuous restructuring of economic relationships have significantly increased global demand for efficient transportation systems. In this context, accurate prediction of the Rate of Penetration (ROP) of the Tunnel Boring Machine (TBM) is crucial for construction planning, cost estimation, and real-time operational decision-making in TBM tunneling. When TBMs are appropriately selected in terms of type and capacity according to route conditions and are operated in compliance with sound engineering principles, they enable the excavation of tunnels at very high rate of penetration while maintaining economic feasibility. Estimating tunnel completion time based on geological and geotechnical conditions along the tunnel alignment and the operational capacity of the TBM has been one of the most intensively studied topics in tunneling research over the past two decades. However, recent advances in artificial intelligence (AI) techniques offer significant potential for achieving higher predictive performance in ROP estimation. In light of these developments, this study evaluates the performance of various AI algorithms using data obtained from the T2 tunnel of the Bahçe–Nurdağ (Türkiye) twin tunnels, the longest railway tunnels in Türkiye. In addition, synthetic input parameters were generated to enhance prediction accuracy beyond that achieved in previous studies. The results demonstrate that incorporating these synthetic input parameters leads to improved model performance, with an increase of up to 2.65% in terms of the correlation coefficient. Given the already high predictive capability achieved without synthetic inputs (R² = 0.8637), the improvement obtained in this study (R² = 0.8866) is particularly noteworthy. Overall, the findings indicate that ensemble-based artificial intelligence models incorporating synthetic input data can predict ROP of TBM with very high accuracy, thereby offering a robust and reliable tool for estimating tunnel completion times in TBM tunneling projects.

How to cite: Gokceoglu, C. and Ozcan, A.: Use of Synthetic Input Parameters for Enhancing Prediction Performance of Rate of Penetration of TBM , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2357, https://doi.org/10.5194/egusphere-egu26-2357, 2026.

EGU26-2503 | ECS | Posters on site | NP5.1

 Spatial aggregation of ROC and PR curves 

Romain Pic, Zhongwei Zhang, Johanna Ziegel, and Sebastian Engelke

Receiver Operating Characteristic (ROC) and Precision–Recall (PR) curves are widely used to assess the discrimination ability of forecasts for binary events, such as threshold exceedances or warnings of extreme events. In weather forecasting, forecasts are provided as spatial fields, yielding location-wise ROC and PR curves that are often aggregated to facilitate comparison, although the effect of the aggregation strategy on performance assessment remains poorly understood.

We investigate how different aggregation strategies for ROC and PR curves affect the assessment of discrimination ability. In particular, we identify conditions under which aggregation strategies satisfy two desirable properties for fair comparison: preservation of dominance between forecasts and preservation of concavity of the curves. We review commonly used aggregation approaches from the literature, analyze their theoretical properties, and highlight potential pitfalls that may lead to misleading interpretations. Based on these findings, we provide practical guidelines for the interpretation of aggregated ROC and PR curves. The proposed framework is illustrated using AI-based global weather forecasts, showing how different aggregation strategies can lead to different rankings.

How to cite: Pic, R., Zhang, Z., Ziegel, J., and Engelke, S.:  Spatial aggregation of ROC and PR curves, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2503, https://doi.org/10.5194/egusphere-egu26-2503, 2026.

EGU26-4039 | ECS | Posters on site | NP5.1

A Framework for Explainable AI in Weather Forecasting: Diagnosing Deep Learning Models via Gradient-Based Attributions 

Younes Essafouri, Corentin Seznec, Luciano Drozda, Laure Raynaud, and Laurent Risser

Each day, potentially critical decisions made by governments and organizations depend on accurate weather forecasts, determining whether to evacuate for a storm or simply to carry an umbrella. In this context, Deep Learning (DL) models are becoming a popular and computationally efficient alternative to traditional Numerical Weather Prediction (NWP) models, offering the potential to capture complex data patterns which may be missed using physical explicit equations (Lam et al., 2023). However, their opaque (black-box) nature remains a barrier to operational trust.

Explainable AI (XAI) aim to address this opacity by revealing the decision process behind predictions. Indeed, classical XAI techniques reveal when DL models rely on spurious correlations rather than causal physical mechanisms to deliver predictions (Geirhos et al., 2020). However, their direct application to meteorological data often yields attribution maps that are noisy (Kim et al., 2019) and difficult to interpret due to their high dimensionality. It additionally remains unclear whether these tools can consistently identify the complex physical drivers inherent in NWP (Bommer et al., 2024).

Based on previous works (Bommer et al., 2024; Kim et al., 2023; Yang et al., 2024), we establish a framework to generate compact and interpretable explanations of local weather forecast predictions obtained using deep neural networks. These explanations build on the output of gradient-based methods like VanillaGrad and SmoothGrad (Smilkov et al., 2017), which are scalable to high-dimensional data. More specifically, our framework first allows for targeted analysis by selecting a region of interest (e.g., Paris area) and a target variable (e.g., accumulated precipitation). It therefore answers the question: "Why did the neural network predict this feature at this location?" To do so, it first computes dense attribution maps with respect to all input variables (e.g., wind components at varying altitudes). Traditionally, bounding boxes are used to define the region of importance in these maps (Kim et al., 2023). However, they are unable to provide detailed directional information. We therefore propose in our framework to determine regions of importance using "confidence ellipses" that summarize the center, main directions, and importance of the most concentrated regions. Unlike bounding boxes, the representation of these ellipses, with the raw attribution maps as a background, provides rich and easily interpretable information regarding the directionality and spatial spread of the model's focus.

Preliminary results on the hybrid transformer-convolutional-based model UNETR++ (Shaker et al., 2024) trained and tested on the TITAN dataset from Météo-France (comprising hourly surface and vertical profiles of wind, temperature, and geopotential over metropolitan France) demonstrate our framework's pertinence for explaining predictions from deep neural networks. We were able to verify that different trained models successfully capture the vertical hierarchy of atmospheric variables, evidenced by an effective receptive field that expands with increasing altitude. More interestingly, our framework allowed us to identify systematic biases learned during training that correlate with known physical occurrences. These findings serve as a foundational step for future work on developing novel explainability methods to detect whether trained models capture complex physical mechanisms.

How to cite: Essafouri, Y., Seznec, C., Drozda, L., Raynaud, L., and Risser, L.: A Framework for Explainable AI in Weather Forecasting: Diagnosing Deep Learning Models via Gradient-Based Attributions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4039, https://doi.org/10.5194/egusphere-egu26-4039, 2026.

Artificial intelligence (AI) and machine learning (ML) tools are rapidly growing in capability and application across the weather enterprise.  Fully AI-based numerical weather prediction (NWP) emulators are beginning to outperform traditional NWP, and many weather agencies have started to adopt ML-derived guidance products into the forecast process.  For example, the United States National Weather Service’s Storm Prediction Center (SPC) has implemented a number of ML models to aid in the prediction and detection of tornadoes, severe wind, hail, and wildfires.  However, the development of these AI/ML products and their subsequent transition into SPC operations revealed several challenges which potentially slowed their overall adoption into the forecasters’ workflow.  This presentation will discuss several factors that impacted the adoption of AI/ML into forecast operations and highlight some best practices used by SPC to help streamline the research-to-operations transition.  Case studies of AI/ML projects that were successfully transitioned into SPC operations will help illustrate the application of these best practices and showcase some of the common pitfalls faced by AI/ML development for operational applications.

How to cite: Harrison, D., Jirak, I., and Marsh, P.: Lessons Learned from the Development and Implementation of AI Forecast Guidance at the U.S. National Weather Service’s Storm Prediction Center, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4103, https://doi.org/10.5194/egusphere-egu26-4103, 2026.

EGU26-4550 | ECS | Orals | NP5.1

From Forecast Skill to Forecast Value: Do AI Weather Forecasts Deliver Real-World Economic Benefits? 

Leonardo Olivetti, Gabriele Messori, Paolo Avner, and Stéphane Hallegatte
Recent years have witnessed rapid advances in data-driven weather forecasting, with an ever-increasing number of AI-based models reporting skill comparable to or exceeding that of physical models. Comparing AI and physical forecasting systems, however, remains challenging: these models often exhibit a different set of strengths and weaknesses, making their real-world value strongly dependent on the specific application. Yet, most existing comparisons of AI and physical models focus exclusively on meteorological skill, largely overlooking the question of forecast value in real-world decision-making.
 
In this talk, we tackle this question by proposing an application-dependent framework to evaluate the real-world value of AI weather forecasts. The framework is based on the classical concept of relative economic value, which we extend in several novel ways to better reflect realistic use cases. Besides allowing for varying cost–loss ratios to represent different protection and forecast costs, we introduce flexible penalty functions to account for compounding losses from sequential forecast misses as well as declining user trust due to repeated false alarms.
 
We apply the framework to a number of case studies, comprising cities exposed to high economic losses from weather-related natural hazards. We show that forecast value in these contexts depends not only on forecast and prevention costs, but also on the choice of penalty function and on whether compound losses from repeated misses or false alarms are considered. We thus advocate for evaluating real-world value alongside meteorological skill when developing and comparing forecasting models, to ensure that improvements in predictive accuracy translate into meaningful societal and economic benefits.

How to cite: Olivetti, L., Messori, G., Avner, P., and Hallegatte, S.: From Forecast Skill to Forecast Value: Do AI Weather Forecasts Deliver Real-World Economic Benefits?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4550, https://doi.org/10.5194/egusphere-egu26-4550, 2026.

Accurate real-time tracking of infectious diseases is often challenged by reporting delays. Existing nowcasting methods typically struggle with three major limitations: they either (1) oversimplify complex reporting delays; (2) ignore spatial connections by treating regions separately; or (3) are too computationally expensive when handling detailed spatio-temporal data, making them impractical for real-time use.

To solve these issues, we propose a flexible Bayesian spatio-temporal framework that incorporates a delay adjustment structure, allowing the framework to adapt to changing reporting behaviors while effectively capturing spatial dependencies. To ensure this complex model is fast enough for real-time applications, we implement it via inlabru using a novel linear approximation strategy. This method significantly improves computational efficiency, enabling scalable inference without the speed bottlenecks of traditional MCMC methods.

We validate the framework by monitoring dengue in Brazilian states during 2025. Our model outperforms the baseline model in 22 out of 26 states (85\% win rate), successfully capturing rapid trend shifts and providing more precise estimates compared to existing systems.

Our findings demonstrate that combining detailed delay dynamics with a spatio-temporal structure effectively balances model flexibility with computational speed. This offers a robust, scalable solution for monitoring epidemics in diverse geographical regions.

How to cite: Xiao, Y. and Moraga, P.: Bayesian spatio-temporal disease nowcasting using parametric time-varying functions of cumulative reporting probability, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4713, https://doi.org/10.5194/egusphere-egu26-4713, 2026.

Multi-step time series forecasting is a fundamental problem across geoscientific applications, including meteorology, hydrology, climate analysis, and space and environmental sciences. A persistent challenge in such tasks is the progressive degradation of predictive accuracy as the forecast horizon increases. This phenomenon is primarily driven by the accumulation and temporal propagation of forecast errors, while most existing statistical and machine learning models lack explicit mechanisms to characterize, model, and correct the evolving dynamics of horizon-dependent residuals.

To address this limitation, we propose an adaptive error post-processing framework termed the Adaptive Residual Decay Mechanism (ARDM). ARDM is designed as an end-to-end predictive optimization strategy that enhances forecasting stability, robustness, and generalization across diverse temporal patterns and application scenarios. Rather than modifying the internal structure of forecasting models, ARDM operates as a residual-aware modification layer that can be seamlessly integrated with a wide range of statistical and machine-learning-based forecasting pipelines.

The proposed framework systematically integrates data preprocessing, initial multi-step forecasting, residual sequence construction, residual dependency modeling, dynamic error modification, and final output refinement. By explicitly constructing residual time series from preliminary forecasts, ARDM captures both short-term and long-term temporal dependencies in forecast errors, enabling structured modeling of error evolution across lead times. Within a symmetrical residual modeling architecture, a time-sensitive adaptive decay function is introduced to dynamically estimate and correct horizon-dependent forecast errors, allowing error adjustments to evolve consistently with increasing prediction horizons.

The decay function and its parameters are optimized through a joint multi-metric loss formulation evaluated across geoscientific and cross-domain time series forecasting datasets. This optimization strategy balances sensitivity to error magnitude with robustness to directional deviations, ensuring stable and reliable post-processing behavior, particularly for longer-range forecasts. Furthermore, ARDM systematically exploits historical residual information during the observation phase, enabling horizon-aware and dynamically consistent refinement of prediction errors through structured residual dependencies without increasing model complexity.

Extensive experiments conducted on multiple real-world geophysical time series datasets, including representative geomagnetic indices, demonstrate that ARDM consistently outperforms mainstream baseline statistical and machine learning methods across a range of standard evaluation metrics, including MAE, MSE, RMSE, MAPE, SSE, and the index of agreement (IA). Performance improvements are especially pronounced at longer prediction horizons, highlighting ARDM’s effectiveness in mitigating error accumulation in multi-step forecasting of geophysical processes. These results suggest that residual-aware, horizon-adaptive statistical post-processing provides a powerful and flexible pathway for improving the reliability of geophysical time series forecasting, with direct relevance to space weather and broader Earth system applications.

How to cite: zhang, Y., zou, Z., and liu, Y.: ARDM: Adaptive Residual Decay Mechanism for Dynamic Error Modification in Geophysical Time Series Forecasting, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4804, https://doi.org/10.5194/egusphere-egu26-4804, 2026.

EGU26-5091 | Posters on site | NP5.1

Fair logarithmic score 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 logarithmic score and are interested in the specific case when the density is multivariate normal with mean and covariance structure given by the ensemble mean and ensemble covariance matrix, respectively. Under the assumptions of multivariate normality and exchangeability of the ensemble members, a relationship is derived that describes the dependence on ensemble size. It is exploited to introduce a fair logarithmic score for multivariate ensemble forecasts [1].

An application to medium-range weather forecasts demonstrates the usefulness of the ensemble size adjustments when multivariate normality is only an approximation, where we consider ensemble predictions of sizes from 8 to 100 of vectors consisting of several different combinations of upper air variables. We show how the logarithmic score depends on ensemble size for various examples and to what extent the fair logarithmic score reduces this dependence.

References

1. Leutbecher, M. and Baran, S., Ensemble size dependence of the logarithmic score for forecasts issued as multivariate normal distributions. Q. J. R. Meteorol. Soc. 151 (2025), paper e4898, doi:10.1002/qj.4898.

*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 logarithmic score for multivariate Gaussian forecasts, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5091, https://doi.org/10.5194/egusphere-egu26-5091, 2026.

A widely recognized limitation of most post-processing methods is that they are typically applied independently for each forecast horizon, location, and variable, potentially neglecting important dependencies across these dimensions. Despite the development of numerous statistical and machine learning methods for modeling these dependencies, the topic remains the subject of ongoing research.
In this work, the proposed approach employs a graph neural network (GNN) trained with a composite loss function that combines the energy score (ES) and the variogram score (VS) for the multivariate postprocessing of ensemble forecasts. The method is evaluated using WRF-based solar irradiance forecasts over northern Chile and ECMWF visibility forecasts over Central Europe.
Across all multivariate verification metrics, the dual-loss GNN consistently outperforms empirical copula–based postprocessing methods as well as GNNs trained solely with CRPS or ES. For the WRF forecasts, the learned rank-order structure captures dependency information more effectively, leading to improved restoration of spatial relationships compared with both the raw ensemble and historical observational ranks. Moreover, incorporating VS into the training loss also improves univariate predictive performance for both forecast targets.

Lakatos, M. (in press). A composite-loss graph neural network for the multivariate post-processing of ensemble weather forecasts.
Quarterly Journal of the Royal Meteorological Society.

How to cite: Lakatos, M.: A Composite-Loss Graph Neural Network for the Multivariate Post-Processing of Ensemble Weather Forecasts , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5377, https://doi.org/10.5194/egusphere-egu26-5377, 2026.

Fog and low stratus forecasting remains a challenge due to the high sensitivity of these phenomena to boundary layer processes. One-dimensional models, such as COBEL–ISBA, offer physical consistency but often lead to systematic errors in key surface variables. This work proposes a novel hybrid calibration framework combining physical modeling with machine learning (ML) to correct COBEL–ISBA forecasts at Nouasseur Airport, Morocco. Using two winter seasons of model outputs and SYNOP observations, we calibrate five variables (2-m temperature and humidity, 10-m wind components, visibility) for each forecast run and lead time (0–12 h).

Two ML architectures are tested: direct correction (ML–COBEL) and residual-learning approach (ML–Phys) using Random Forest and XGBoost. For visibility, a two-stage classification-regression model is implemented, and an oversampling technique is used to address class imbalance. Results are benchmarked against classical bias correction and quantile mapping.

The ML–Phys approach outperforms traditional methods across all variables and lead times, reducing errors (bias, RMSE) while preserving observed temporal variability. Furthermore, it improves also low-visibility event detection. In contrast, traditional methods show limited skill, often degrading beyond short lead times. This work demonstrates the potential of hybrid AI-physics strategies to mitigate 1D model limitations, providing a path toward more reliable operational fog and visibility forecasting.

How to cite: Oubouisk, M., Bari, D., and Mordane, S.: Hybrid AI-Physics Calibration of a 1D Fog Model: Improving Near-Surface and Visibility Forecasts at a Moroccan Airport, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5760, https://doi.org/10.5194/egusphere-egu26-5760, 2026.

EGU26-7223 | ECS | Orals | NP5.1

How skilful are AI-based forecasts of 2023 Indian summer monsoon precipitation? 

Mehzooz Nizar, Reinhard Schiemann, Andrew G Turner, Kieran Hunt, and Steffen Tietsche

India relies on agriculture as one of its main sources of income. Therefore, reliable prediction of Indian summer monsoon
rainfall is crucial to the country’s policy making and development of crop management strategies. The recent development
of global AI Weather Prediction (AIWP) models has revolutionized weather forecasting. Owing to the very recent
emergence of AIWP models, their performance in simulating the Indian monsoon system is still insufficiently explored.
In this study, we verify the precipitation forecast skill of AIWP models GraphCast and FuXi at a lead time of 1-9 days
during Indian summer monsoon 2023 and compare their performance to the physics-based model ECMWF IFS-HRES
(IFS). Satellite-derived precipitation dataset IMERG is used as the ground truth to verify precipitation along with
ERA5 precipitation. Root mean squared error (RMSE), pattern correlation coefficient (PCC), structure (S)-amplitude
(A)-location error (L) and stable equitable error in probability space (SEEPS) were the metrics used to evaluate the
models.

A number of case studies, seasonal and intra-seasonal characteristics of precipitation forecast at various lead times were
analysed during June-September 2023. The case studies reveal that the AIWP models have lower RMSE and higher PCC
than IFS in general, while the AIWP models smoothen (positive S error) precipitation at longer leads. FuXi consistently
underestimates precipitation (negative A error) in the case studies. Analysing the daily mean rainfall for the country
as a whole and the precipitation bias at a lead time of 5 days, it is confirmed that FuXi shows a systematic dry bias in
forecasting monsoon rainfall. Non-parametric statistical tests were conducted to decide which model performs the best
at each metric in forecasting the entire season at various lead times. It is found that FuXi consistently achieved the
lowest RMSE, IFS delivered the best S, and GraphCast recorded the smallest SEEPS score at a lead time of 1, 5 and 9
days while no model shows a significant advantage in PCC, A and L. It was also seen that AIWP models outperformed
IFS in RMSE and PCC while AIWP models have larger S error than IFS corroborating the findings of case studies.
FuXi scored the largest A error across all lead times. The loss functions used to train AIWP models directly penalise
point-wise errors, which likely explains their RMSE advantage over IFS.

These results show us that even though AIWP models have good overall accuracy and correlation with observed precipi-
tation, exhibits a lack of realism in capturing the spatial distribution and the intensity of precipitation. Also, model skill
is metric dependent and choosing between an AIWP or physics-based model should hinge on the forecaster’s priority.

How to cite: Nizar, M., Schiemann, R., Turner, A. G., Hunt, K., and Tietsche, S.: How skilful are AI-based forecasts of 2023 Indian summer monsoon precipitation?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7223, https://doi.org/10.5194/egusphere-egu26-7223, 2026.

EGU26-7775 | ECS | Posters on site | NP5.1

Advancing Rainfall Nowcasting in Tropical Southeast Asia with Physics-Informed Deep Generative Models 

Zhixiao Niu, Song Chen, Zhihuo Xu, Joshua Lee, Hugh Zhang, Shuping Ma, Yaomin Wang, Xinyue Liu, and Xiaogang He

Rainfall nowcasting of deep convection in the tropics is extremely challenging, particularly in highly urbanized coastal regions such as Singapore, where high spatial resolution is required. Conventional optical flow-based nowcasting methods typically struggle with capturing the initiation, duration, and spatiotemporal evolution of deep convection and rainfall. When it comes to extreme rainfall, these existing methods cannot deliver skillful nowcasts due to rapid changes in localized features of individual deep convection events. Recent advances in AI-based data-driven models, particularly deep generative models utilizing high-resolution radar imagery, have improved nowcasting accuracy at longer lead times. However, they often serve as black boxes, neglecting the underlying physics, potentially missing unseen extremes, and underestimating their rainfall intensity. To better tackle convection onset prediction, we adopt a novel importance sampling strategy that targets convective initiation by identifying convective cells based on a 35 dBZ threshold and fitting a linear growth trend across frames. Samples with steeper growth and fewer initial convective cells are prioritized to emphasize early-stage development. To enhance physical realism in deep tropics, we further propose a physics-informed deep generative model that incorporates diurnal and seasonal cycles to reflect tropical weather variability. Moreover, the model includes three-dimensional physical information such as Doppler wind and multi-altitude reflectivity. With the incorporation of additional physical information, the proposed generative framework consistently outperforms baseline models, particularly at early forecast lead times. Relative to the original DGMR driven solely by precipitation inputs, the physics-informed model achieves substantially higher skill across multiple rainfall thresholds. Over a 90-min forecast horizon, the average probabilities of detection (POD) reach 0.70, 0.47, and 0.21 at 1.0, 4.0, and 16.0 mm h⁻¹, corresponding to relative improvements of 27%, 25%, and 25%, respectively, with associated critical success indices (CSI) of 0.47, 0.30, and 0.15. In addition, spatial correlation is enhanced across pooling scales of 0.5, 2.0, and 8.0 km, yielding average Pearson correlation coefficients (PCC) of 0.27, 0.32, and 0.46, representing relative gains of 15–16% compared with the baseline. Attribution analysis further indicates that multi-altitude reflectivity contributes most strongly to nowcasting skill, followed by composite reflectivity, while the influence of time-regime information increases with forecast lead time and the contribution of three-dimensional wind fields remains comparatively modest. Our novel physics-informed deep generative model provides valuable insight into convective precipitation processes, supports more reliable nowcasting, and helps guide future data collection in tropical regions.

How to cite: Niu, Z., Chen, S., Xu, Z., Lee, J., Zhang, H., Ma, S., Wang, Y., Liu, X., and He, X.: Advancing Rainfall Nowcasting in Tropical Southeast Asia with Physics-Informed Deep Generative Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7775, https://doi.org/10.5194/egusphere-egu26-7775, 2026.

EGU26-7988 | ECS | Orals | NP5.1

Assessment of high-resolution physical and AI-based precipitation forecasts in the Ecuadorian Tropics 

Angela Iza-Wong, Gabriel Moldovan, Zied Ben Bouallegue, Becky Hemingway, Matthew Chantry, and David A. Lavers

Accurate precipitation forecasting remains challenging, particularly in regions with complex terrain and sparse observational networks. This study evaluates precipitation forecasts from the European Centre for Medium-Range Weather Forecasts (ECMWF), the Integrated Forecasting System (IFS), and Artificial Intelligence/Integrated Forecasting System (AIFS) (ECMWF, 2024, 2025)​, including experimental models trained on the Integrated Multi-satellite Retrievals for GPM (IMERG) and Multi-Source Weighted-Ensemble Precipitation (MSWEP) datasets, the high-resolution (4km) model developed within the Destination Earth (DestinE) initiative (ECMWF et al., 2025)​, and the GraphCast model (Lam et al., 2022)​. The evaluation is based on 2 years of observational data (2023–2024) from 30 Ecuadorian weather stations in coastal and Andean regions and considers forecast lead times of 1-10 days. Throughout the evaluation period, AIFS exhibits the highest overall predictive skill, whereas DestinE is most effective at identifying extreme precipitation events. Most models display a marked positive bias, particularly within the Andean region. AIFS models trained on IMERG and MSWEP demonstrate the lowest bias and highest skill, as indicated by the Stable Equitable Error in Probability Space (SEEPS) ​(Rodwell et al., 2010)​ and the Equitable Threat Score (ETS). The Frequency Bias Index (FBI) decreases across all models as thresholds increase from the 90th to the 99th percentile, with consistently elevated FBI values observed over mountainous terrain. AIFS (IMERG) achieves the best overall performance, while GraphCast demonstrates the lowest skill in both total and mountainous regions. Overall, in the Ecuadorian tropics, AI-based models generally outperform physical models, except during extreme precipitation events, when physical models remain more reliable. These results underscore the critical importance of training data for AI-based systems and the ongoing challenges of forecasting high-impact precipitation across both operational and experimental models.

Keywords: Precipitation forecasting, artificial intelligence, ECMWF, GraphCast, Ecuador, extreme rainfall

References

ECMWF. (2024). IFS Documentation CY49R1 - Part I: Observations. In IFS Documentation CY49R1. ECMWF. https://doi.org/10.21957/fd16c61484

ECMWF. (2025). ECMWF’s AI forecasts become operational ECMWF. https://www.ecmwf.int/en/about/media-centre/news/2025/ecmwfs-ai-forecasts-become-operational

ECMWF, EUMETSAT, & ESA. (2025). Destination Earth (DestinE)-digital model of the Earth. https://destination-earth.eu/

Lam, R., Sanchez-Gonzalez, A., Willson, M., Wirnsberger, P., Fortunato, M., Alet, F., Ravuri, S., Ewalds, T., Eaton-Rosen, Z., Hu, W., Merose, A., Hoyer, S., Holland, G., Vinyals, O., Stott, J., Pritzel, A., Mohamed, S., & Battaglia, P. (2022). GraphCast: Learning skillful medium-range global weather forecasting. http://arxiv.org/abs/2212.12794

Rodwell, M. J., Richardson, D. S., Hewson, T. D., & Haiden, T. (2010). A new equitable score suitable for verifying precipitation in numerical weather prediction. Quarterly Journal of the Royal Meteorological Society, 136(650), 1344–1363. https://doi.org/10.1002/qj.656

How to cite: Iza-Wong, A., Moldovan, G., Bouallegue, Z. B., Hemingway, B., Chantry, M., and Lavers, D. A.: Assessment of high-resolution physical and AI-based precipitation forecasts in the Ecuadorian Tropics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7988, https://doi.org/10.5194/egusphere-egu26-7988, 2026.

EGU26-8100 | Posters on site | NP5.1

COBASE: A new copula-based shuffling method for ensemble weather forecast postprocessing 

Elisa Perrone, Maurits Flos, Bastien François, Irene Schicker, and Kirien Whan

Weather predictions are often provided as ensembles generated by repeated runs of numerical weather prediction models. These forecasts typically exhibit bias and inaccurate dependence structures due to numerical and dispersion errors, requiring statistical postprocessing for improved precision. A common correction strategy is the two-step approach: first adjusting the univariate forecasts, then reconstructing the multivariate dependence. The second step is usually handled with nonparametric methods, which can underperform when historical data are limited. Parametric alternatives, such as the Gaussian Copula Approach (GCA), offer theoretical advantages but often produce poorly calibrated multivariate forecasts due to random sampling of the corrected univariate margins. In this work, we introduce COBASE, a novel copula-based postprocessing framework that preserves the flexibility of parametric modeling while mimicking the nonparametric techniques through a rank-shuffling mechanism. This design ensures calibrated margins and realistic dependence reconstruction. We evaluate COBASE on multi-site 2-meter temperature forecasts from the ALADIN-LAEF ensemble over Austria and on joint forecasts of temperature and dew point temperature from the ECMWF system in the Netherlands. Across all regions, COBASE variants consistently outperform traditional copula-based approaches, such as GCA, and achieve performance on par with state-of-the-art nonparametric methods like SimSchaake and ECC, with only minimal differences across settings. These results position COBASE as a competitive and robust alternative for multivariate ensemble postprocessing, offering a principled bridge between parametric and nonparametric dependence reconstruction.

How to cite: Perrone, E., Flos, M., François, B., Schicker, I., and Whan, K.: COBASE: A new copula-based shuffling method for ensemble weather forecast postprocessing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8100, https://doi.org/10.5194/egusphere-egu26-8100, 2026.

EGU26-8449 | Orals | NP5.1

High-resolution Probabilistic Forecasts of Fire Weather Conditions in California using Downscaling Machine Learning Models 

Charles Jones, Callum Thompson, David Siuta, Nathan Quinn, and Nicholas Sette

California is prone to extreme fire weather conditions characterized by high winds, elevated temperatures, and low humidity. Accurate predictions with high spatial resolution are critical for emergency operations to monitor and respond to fast-spreading wildfires. While current operational numerical weather prediction models, such as the NOAA Global Forecasting System GFS model, offer reliable probabilistic forecasts in the medium range (up to 15 days), their coarse spatial resolution (typically 0.25° latitude/longitude, ~25 km) limits their utility for localized fire risk assessment. This resolution is insufficient for capturing terrain-driven wind patterns and microclimate variations that drive fire behavior, especially in complex topography regions like the wildland–urban interface.

High-resolution probabilistic forecasts of fire weather conditions are generated by downscaling GFS ensemble outputs from a native resolution of 0.25° latitude/longitude to 1.5 km horizontal grid spacing over a domain encompassing California and Nevada. The downscaling framework integrates singular value decomposition (SVD), UNet-based convolutional neural networks, and diffusion models to capture both large-scale variability and fine-scale terrain-driven features. Models are trained using GFS initial conditions (00 UTC) and paired with 1.5 km Weather Research and Forecasting (WRF) simulations spanning the period 2015–2020. To evaluate forecast skill, ten high-impact case studies characterized by strong wind events in the Sierra Nevada and Southern California are analyzed. Probabilistic predictions of surface air temperature, relative humidity, and wind speed are validated against surface meteorological observations. The study includes a discussion of forecast skill metrics, operational applications, and ongoing research directions.

How to cite: Jones, C., Thompson, C., Siuta, D., Quinn, N., and Sette, N.: High-resolution Probabilistic Forecasts of Fire Weather Conditions in California using Downscaling Machine Learning Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8449, https://doi.org/10.5194/egusphere-egu26-8449, 2026.

EGU26-8532 | ECS | Orals | NP5.1

Design, operation and validation of the ERA5-land Global Gridded Stochastic Weather Generator 

Alex Schuddeboom, Christian Zammit, David Plew, Piet Verburg, and Aidin Jabbari

The ERA5-land Global Gridded Stochastic Weather Generator (EGGS-WG) model was released to the public last year as an open source and freely accessible stochastic weather generator. The purpose of this model is to provide an easy to use, low resource and modern Stochastic Weather Generator that can produce rainfall, air temperature and dew point temperature. This model offers several advancements over existing freely available stochastic weather generators, including the ability to simulate any terrestrial region of the planet, moving from a single site simulation approach to an entire gridded domain and increasing the temporal resolution of temperature simulation from daily to hourly.

Validation case studies have been performed over a range of different regions that represent substantially different climates. In general, EGGS-WG shows a strong ability to recreate the statistical behaviour seen in the ERA5-Land dataset. Precipitation occurrence rates and daily rainfall amounts are shown to be reproduced accurately by the model. Several different aspects of these variables are validated, including seasonality, spatial correlations and rainfall spells. While the general quality of the simulation is high, there are some clear issues in the simulation of the most extreme precipitation values, as well as some unique issues in consistently wet climates. Analysis of the air temperature and dew point temperature simulations shows stronger agreement. In particular, the spatial distributions and diurnal cycles of temperature are shown to be well simulated.

Many future developments have been planned that build on the released software package. Most prominent amongst these is the expansion of the simulated variables to include winds and radiation, which introduces a unique set of challenges due to the strong diurnal patterns and spatial organisation. Additionally, integrated support for CMIP6 driven future warming simulation is a high priority. These extensions are in various stages of development and are likely to be released over the coming year.

How to cite: Schuddeboom, A., Zammit, C., Plew, D., Verburg, P., and Jabbari, A.: Design, operation and validation of the ERA5-land Global Gridded Stochastic Weather Generator, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8532, https://doi.org/10.5194/egusphere-egu26-8532, 2026.

EGU26-8733 | Orals | NP5.1

Development of AI-based precipitation forecasting at KIAPS 

Tae-Jin Oh, In-Chae Na, and Woo-Yeon Park

This study outlines the development of an artificial intelligence (AI)-based precipitation forecasting system at the Korea Institute of Atmospheric Prediction Systems (KIAPS). The system is designed with three main components:  an observation-based model for very short-term forecasting (nowcasting), a post-processing model to correct numerical weather prediction (NWP) fields for longer lead times, and a hybrid model to integrate these approaches which is to be built. The nowcasting model utilizes a U-Net architecture incorporating ConvLSTM at the bottleneck. It uses radar and satellite data sequences to produce 6-hour forecasts; the training strategy involves pretraining on radar/satellite data followed by fine-tuning with 1-hour accumulated rainfall gauge data from Automatic Weather Stations (AWS). The post-processing model employs a ConvNeXt v2 U-Net to correct Korea Integrated Model (KIM) NWP fields for forecasts up to 24 hours. Performance evaluations show that the observation-based model excels at shorter lead times with 34% improvement in the Critical Success Index (CSI) for precipitation exceeding 8 mm/hr, averaged over the 1–6 hour forecast period, compared to the baseline KIM forecast. Meanwhile, the post-processing model, which incorporates a differentiable CSI loss function for robust heavy precipitation forecasting, averaged over the 24 hour forecast period, achieves 31% CSI improvement relative to KIM with reduced performance degradation at longer lead times. Future work will focus on developing the hybrid model to merge these outputs for optimal accuracy across all forecast lead times.

How to cite: Oh, T.-J., Na, I.-C., and Park, W.-Y.: Development of AI-based precipitation forecasting at KIAPS, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8733, https://doi.org/10.5194/egusphere-egu26-8733, 2026.

EGU26-9336 | Posters on site | NP5.1

Environment-Specific Fog Detection over the Korean Peninsula Using GEO-KOMPSAT-2A and DeepLabV3+ 

Suhwan Kim, Dongjin Kim, and Jong-Min Yeom

Fog detection using geostationary satellite data has the advantage of monitoring large areas in a short period of time. However, because fog exhibits highly diverse optical characteristics in both space and time, it is difficult to achieve reliable detection with a single satellite-based detection strategy that does not consider environmental conditions. Therefore, this study utilized data from GEO-KOMPSAT-2A (GK2A) to pre-define fog occurrence environments, construct appropriate input data and labels for each environmental condition, and then applied a categorized deep learning-based fog detection system.

First, fog was identified when ground-station visibility was under 1 km. To create reliable training data, the ground-station visibility data was spatially aligned with fog labels from the Korea Meteorological Administration (KMA) for GK2A observations. Only areas consistently identified as fog by both ground-station observations and KMA fog labels were selected and cropped. In this process, a spatial grouping method was used to eliminate noise and ensure the fog regions had continuous spatial coverage.        

In constructing the input data, variables representing surface characteristics were chosen to optimize detection accuracy for each environmental condition. Using this high-quality dataset, data were organized into different groups based on four seasons, three time periods (daytime, nighttime, dawn/dusk), and two surface types (land, ocean). Separate DeepLabV3+ models were trained for each category, with 2022 data used for training and 2023 data for validation.

To evaluate the model's ability to generalize, the entire 2024 dataset not included in training was used as an independent test set. For accurate assessment, post-processing filtering with a cloud mask was applied to measure detection performance in cloud-free regions. The results revealed notable seasonal fluctuations in performance, indicating that detection efficiency depends on environmental conditions. Even with the same deep learning architecture, this suggests that careful data preprocessing and environment-specific strategies can help advance satellite-based fog detection technology.

 

This work was supported by the National Research Foundation of Korea(NRF) grant funded by the Korea government(MSIT)(RS-2025-00515357).

How to cite: Kim, S., Kim, D., and Yeom, J.-M.: Environment-Specific Fog Detection over the Korean Peninsula Using GEO-KOMPSAT-2A and DeepLabV3+, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9336, https://doi.org/10.5194/egusphere-egu26-9336, 2026.

EGU26-9685 | ECS | Orals | NP5.1

Comparative Assessment of Predictor Variable Combinations within Data Driven Approaches for NWP based Precipitation Forecast Enhancement 

Sudhanyasree Prasanna Ravikumar, Sakila Saminathan, and Subhasis Mitra

Precipitation forecasts generated by Numerical Weather Prediction (NWP) models often exhibit systematic biases arising from limitations in model resolution, representation of sub-grid-scale processes, and uncertainties in initial conditions. This study systematically assesses different predictor combinations (PC) obtained from the European Centre for Medium-Range Weather Forecasts (ECMWF) model to improve short-range precipitation forecasts using data-driven approaches over the peninsular Indian region. Different data-driven formulations, comprising of four machine learning (ML) models and two deep learning (DL) models, were implemented and systematically compared. Further, the different PCs and data driven formulations are evaluated and compared against the traditional Bayesian Model Averaging (BMA) approach, widely adopted for precipitation forecast enhancement. The improvement in precipitation forecast skill was assessed using standard deterministic and probabilistic verification metrics. The results indicate that incorporating exogenous predictor variables leads to a slight improvement in precipitation forecast skill, while DL models exhibit performance comparable to that of traditional ML models. Overall, the exogenous variable PC achieved higher forecast skill than other PCs and the traditional BMA, yielding an approximate 20% improvement in RMSE compared to 14% for the traditional BMA. Feature importance analysis revealed that total precipitation, wind speed, and 2-m temperature consistently ranked among the top five most influential variables across the different data driven formulations, underscoring the interpretability of the models.

How to cite: Prasanna Ravikumar, S., Saminathan, S., and Mitra, S.: Comparative Assessment of Predictor Variable Combinations within Data Driven Approaches for NWP based Precipitation Forecast Enhancement, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9685, https://doi.org/10.5194/egusphere-egu26-9685, 2026.

EGU26-10414 | Orals | NP5.1

Forecasting Cold Winter Temperatures in Finland with the Aila AI Weather Model 

Marko Laine, Leila Hieta, Tuukka Tuukka Himanka, Mikko Partio, and Olle Räty

Advances in data-driven artificial intelligence (AI) weather models are transforming how national meteorological services produce forecasts. The Finnish Meteorological Institute (FMI) has developed Aila, a regional AI model inspired by Met Norway's Bris AI model and built using the Anemoi framework - an open European initiative that integrates machine learning techniques with meteorology. Aila has been trained on 40 years of European Centre for Medium-Range Weather Forecasts (ECMWF) global historical ERA5 reanalysis data and about three years of high-resolution Harmonie analyses over the Scandinavian region, utilizing the computational power of the LUMI supercomputer. The model's graph-based neural network architecture enables enhanced spatial resolution and improved representation of atmospheric processes over Northern Europe. 

This study focuses on evaluating Aila's performance during cold winter conditions in Finland, a key challenge for numerical weather prediction models. Prolonged low-temperature episodes are often governed by persistent high-pressure systems and strong temperature inversions that prove difficult to forecast accurately. Using case studies from recent winters, we evaluate Aila’s skill in forecasting 2-meter temperatures during cold spells by comparing its predictions against FMI's operational forecast products and observations.

The results demonstrate that the AI-based Aila model achieves competitive accuracy in temperature forecasts during challenging cold weather conditions while providing substantial computational efficiency compared to traditional numerical approaches. Future development efforts will focus on implementing a multi-decoder approach where the Aila model will be fine-tuned using observational data to better capture extreme cold temperatures and improve forecast reliability.

How to cite: Laine, M., Hieta, L., Tuukka Himanka, T., Partio, M., and Räty, O.: Forecasting Cold Winter Temperatures in Finland with the Aila AI Weather Model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10414, https://doi.org/10.5194/egusphere-egu26-10414, 2026.

EGU26-11641 | ECS | Orals | NP5.1

Hybrid Neural Operator and Physics-Informed Learning for Renewable Energy Forecasting 

Andrejs Cvečkovskis, Juris Seņņikovs, and Uldis Bethers

Forecasting of local renewable energy variables such as solar irradiance and wind speed is critically important for operational grid management and energy markets. We present a hybrid machine learning model that combines Adaptive Fourier Neural Operator (AFNO) architectures with physics-informed loss constraints, designed to capture both learned spatial–temporal patterns and key physical relationships in atmospheric fields. The model is trained on reanalysis and high-resolution observational datasets over the Baltic region and evaluated in comparison with baseline statistical and numerical weather prediction benchmarks.

Our contributions include: (i) a hybrid modelling strategy that enforces approximate physical consistency via penalised residuals of key balance equations during training; (ii) a detailed benchmarking framework for lead-time dependent forecast skill on solar and wind energy generation targets; and (iii) an assessment of uncertainty and calibration properties using probabilistic scoring metrics. Results are evaluated against numerical weather prediction baselines, highlighting the strengths and limitations of the hybrid approach and outlining a viable pathway for future improvements in sub-daily renewable energy forecasting.

This work contributes to the session’s themes of advanced machine learning and statistical forecasting methods in geosciences and highlights the potential of hybrid approaches for enhancing short-term predictive skill.

How to cite: Cvečkovskis, A., Seņņikovs, J., and Bethers, U.: Hybrid Neural Operator and Physics-Informed Learning for Renewable Energy Forecasting, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11641, https://doi.org/10.5194/egusphere-egu26-11641, 2026.

EGU26-11765 | ECS | Orals | NP5.1

Assessing the physical realism of AI-based weather forecasts: insights from extratropical storms and large-scale flow diagnostics. 

Soufiane Karmouche, Linus Magnusson, Tim Hewson, and Thomas Haiden

Standard scores such as the root mean squared error provide limited insight into whether Machine-learning (ML) weather prediction systems reproduce the physically consistent dynamical structures that underpin high-impact weather. Here, we present a multi-faceted assessment of the physical realism of ECMWF’s Artificial Intelligence Forecasting System (AIFS), combining case-study diagnostics of severe extratropical storms with conditional verification based on large-scale circulation.

We first examine two North Atlantic storms: Storm Amy (October 2025) and Storm Eowyn (January 2025). Using diagnostics inspired by Charlton-Perez et al. (2024), we analyse frontal structure, vorticity, and surface and upper-air wind fields in AIFS-Single and AIFS Ensemble Control forecasts, benchmarked against the IFS Control and analysis. While ML systems capture storm tracks and large-scale frontal geometry well, they systematically smooth sharp gradients, compact vorticity cores, and localized wind maxima, leading to underestimation of extreme winds. Probabilistic training in the ensemble configuration improves realism but does not fully overcome these structural limitations.

We then present ongoing work assessing the physical consistency of ML forecasts using diagnostics of the ageostrophic-to-geostrophic wind ratio at multiple pressure levels. These reveal systematic differences between ML-based and physics-based models, particularly in dynamically active midlatitude regions.

Finally, we present regime-based verification results highlighting improved AIFS performance for 2-m temperature forecasts during persistent wintertime anticyclonic conditions, illustrating ML strengths in stable large-scale regimes where physics-based forecasts suffer from long-standing systematic biases.

Overall, our results highlight the importance of moving beyond general verification scores toward diagnostic and physically interpretable evaluation frameworks when assessing AI-based weather forecasts, especially for high-impact weather events.

This work is funded by the Destination Earth project.

REFERENCES:

Charlton-Perez, A.J., Dacre, H.F., Driscoll, S. et al. Do AI models produce better weather forecasts than physics-based models? A quantitative evaluation case study of Storm Ciarán. npj Clim Atmos Sci 7, 93 (2024). https://doi.org/10.1038/s41612-024-00638-w

How to cite: Karmouche, S., Magnusson, L., Hewson, T., and Haiden, T.: Assessing the physical realism of AI-based weather forecasts: insights from extratropical storms and large-scale flow diagnostics., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11765, https://doi.org/10.5194/egusphere-egu26-11765, 2026.

I present a data-driven forecast system applied to the Indian summer monsoon rain. By forecasting pentads, 5-day rain totals, the system is well suited to forecasting the monsoon onset/withdrawal as well as its progression, also known as intra-seasonal variability. I will provide a comparison of the forecast skill with those of other systems, both physics-based NWP and AI systems. The skill of the JJA seasonal forecast issued on 1 May in terms of the Pearson correlation coefficient far surpasses that of GLOSEA5. I will also discuss delicate questions about forecast skill, as to what is concepotually sound and what can be computed.

How to cite: Bodai, T.: Data-driven seasonal weather forecast: An application to the Indian summer monsoon rain, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12477, https://doi.org/10.5194/egusphere-egu26-12477, 2026.

EGU26-12713 | ECS | Posters on site | NP5.1

Verifying the spatial structure of precipitation fields from a foundation model of the atmosphere 

Sebastian Buschow and Wael Almikaeel and the WeatherGenerator Team

Data driven weather models have proven their ability to learn various aspects of the weather prediction problem. While their point-to-point skill has been proven, the precise nature of their errors is not yet fully understood.

This contribution takes a first look at the spatial precipitation patterns simulated by the Weather Generator – a foundation model trained on diverse data sources with the goal of learning the underlying behavior of the atmosphere as a whole.  We analyze the correlation structure of the simulated precipitation fields using spatial verification techniques including two-dimensional wavelet transforms. Some attention is paid to the problem of applying these methods to global data on an irregular grid. The results can be compared to observations, reanalysis and potentially other data-driven forecast models.

How to cite: Buschow, S. and Almikaeel, W. and the WeatherGenerator Team: Verifying the spatial structure of precipitation fields from a foundation model of the atmosphere, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12713, https://doi.org/10.5194/egusphere-egu26-12713, 2026.

EGU26-12781 | Orals | NP5.1

A Lagrangian blending of optical flow and ML-based radar precipitation nowcasts  

Dominique Brunet, Laura Huang, Jonathan Belletête, Ahmed Mahidjiba, and Sudesh Boodoo

Recent research and development at Environment and Climate Change Canada has been conducted on improving the current operational radar precipitation nowcasting by transitioning from an optical flow method (Farnebäck smoothed) to machine learning (ML)-based nowcasts. Two ML-based nowcasting models were trained on the Canadian radar composite: RainNet, a convolutional neural network based on the U-Net architecture, and NowcastNet, which combines a Generative Adversarial Network with an Evolution Network to explicitly model precipitation dynamics. Verification of radar precipitation nowcasts revealed that the optimal method depends on both lead time and precipitation threshold. RainNet performed best for low precipitation thresholds (0.1-1 mm/h) at all lead times, highlighting its ability to capture widespread, weak precipitation, while NowcastNet outperformed the others at longer lead times (beyond one hour) and for higher precipitation thresholds (4+ mm/h). Farnebäck smoothed remained the most skillful for nowcasting heavy precipitation (12+ mm/h) during the first hour, likely due to its robust short-term motion estimation. 

Building on these results, we propose a Lagrangian blending method that optimally combines the predicted motion paths and the growth and decay of precipitation intensity components of the different nowcasting methods.  While optical flow methods assume constant motion and intensity evolution, ML-based methods produce time-varying motion vectors and precipitation intensities, which are explicitly leveraged in the blending framework. For deterministic nowcasts, we apply a bias-correction followed by the blending of both motion paths and intensity, allowing the generation of time-evolving blended motion fields with growth and decay.  

We also generate probabilistic nowcasts of precipitation occurrence (0.1 mm/h) and extreme precipitation (50 mm/h) by determining the optimal spatial smoothing for each model and lead time based on the area under the ROC curve. We then calibrate the resulting probabilities using isotonic (i.e. monotonically increasing) regression. Experiments are conducted using both static and dynamically varying weighting strategies for both deterministic and probabilistic radar precipitation nowcasting. The goal is to produce a blended and post-processed nowcast that outperforms each individual method across all lead times and precipitation thresholds. 

How to cite: Brunet, D., Huang, L., Belletête, J., Mahidjiba, A., and Boodoo, S.: A Lagrangian blending of optical flow and ML-based radar precipitation nowcasts , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12781, https://doi.org/10.5194/egusphere-egu26-12781, 2026.

EGU26-13223 | ECS | Orals | NP5.1

Scale-dependent analysis of the accuracy–activity trade-off in AI weather forecasts 

Britta Seegebrecht, Sabrina Wahl, Stefanie Hollborn, Erik Pavel, Wael Almikaeel, Michael Langguth, Martin Schultz, Christian Lessig, Ilaria Luise, Juergen Gall, Anas Al-Iahham, and Mohamad Hakam Shams Eddin

Data-driven weather prediction models based on artificial intelligence (AI) have rapidly advanced in recent years and are frequently reported to outperform traditional physics-based numerical weather prediction (NWP) models for selected verification scores. However, optimization with respect to a specific loss function can adversely affect other metrics, potentially leading to unrealistic forecast characteristics, such as overly smooth spatial structures when mean-squared or mean-absolute error–based loss functions are used.

A robust and meaningful comparison of AI-based and NWP models therefore requires a carefully chosen and diverse set of verification metrics that accounts for potential dependencies. The main focus is placed on the prominent forecast accuracy-activity tradeoff, associated with the double penalty problem of deterministic forecasts. Related questions include: How sensitive is the relationship between accuracy and activity metrics to the choice of verification measure? Are there systematic differences between AI-based and NWP models? What is the impact of the (in)dependence between the AI training loss function and the verification metrics on the assessment of forecast skill?

These questions are addressed using both scale-independent and scale-dependent verification metrics, allowing the quantification of forecast performance on individual spatial scales.

As a starting point, global deterministic forecasts are considered. The analysis is partly based on forecasts from the Weather Prediction Model Intercomparison Project (WP MIP), which provides a collection of NWP and AI-model forecasts from multiple national weather services and research institutions.

The work is conducted within the RAINA project, which aims to develop a foundation model for the atmosphere with a particular focus on reliable, high-resolution forecasts of extreme wind and precipitation events. Consequently, the relation between, e.g., forecast activity and the predictive capability for extreme weather are of special interest.

How to cite: Seegebrecht, B., Wahl, S., Hollborn, S., Pavel, E., Almikaeel, W., Langguth, M., Schultz, M., Lessig, C., Luise, I., Gall, J., Al-Iahham, A., and Shams Eddin, M. H.: Scale-dependent analysis of the accuracy–activity trade-off in AI weather forecasts, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13223, https://doi.org/10.5194/egusphere-egu26-13223, 2026.

As meteorological organisations transition to high-resolution ensemble-based forecasting, they risk leaving behind downstream users who rely on deterministic data: a need that may arise from the inability to process large volumes of data, or difficulty integrating probabilistic information into decision-making processes. Current solutions for such users typically involve providing the control (unperturbed) member of the ensemble, or deriving a single-value forecast through the independent treatment of variables (e.g., taking a median). However, relying solely on the control member discards the valuable information encoded within the full ensemble, fundamentally undermining the purpose of the ensemble. Meanwhile, univariate approaches can result in forecasts that lack physical consistency across variables. This limitation becomes critical when variables are interpreted jointly in real‑world decision‑making. Wind speed and direction exemplify this: these variables are used together in sectors such as renewable energy, where they inform turbine operation and resource planning, and aviation, where they underpin safety‑critical decisions around take‑off and landing. For these users, unrealistic combinations of speed and direction can translate directly into flawed risk assessments. 

  

To address this gap, we present a novel ensemble post-processing technique that generates physically-consistent spot forecasts of wind speed and direction by exploiting the full ensemble distribution. The method constructs joint predictive probability density functions (PDFs) using a Gamma kernel for wind speed and a von Mises kernel for wind direction, accommodating the distinct statistical properties of these variables: non-negativity and skewness for speed, and circularity for direction. A single-value forecast is then obtained by selecting the ensemble member that maximizes its log-likelihood under the joint density across a specified forecast horizon. Because the selected forecast corresponds to one of the original ensemble members, it represents a physically plausible atmospheric state and maintains consistency across all variables, including those not directly analysed. This is critical for operational users: approaches that treat wind speed and direction separately (such as taking independent averages or applying separate post-processing to each variable) can produce unrealistic artefacts when passed through downstream physical or statistical models.  

  

This method was evaluated using the Met Office convective-scale ensemble, MOGREPS-UK, over the UK domain for a full calendar year, with verification at both the surface and aloft. Results are promising: the approach demonstrates the potential to outperform the control member, particularly at longer leadtimes where ensemble spread is greatest. These findings highlight an important step toward improving our offering to users and ensuring they remain supported as we transition to purely ensemble-based forecasting. Crucially, this work is not just theoretical; the next stage is to embed the technique into operational workflows and deliver it within user-facing products, ensuring these advances translate directly into improved real-world decision-making. 

How to cite: Lake, A.: Joint Forecasting of Wind Speed and Direction via Ensemble Post-Processing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13365, https://doi.org/10.5194/egusphere-egu26-13365, 2026.

Current state-of-the-art artificial-intelligence weather prediction (AI-WP) systems are trained on a large archive of atmospheric reanalysis data. The training objective is to replicate the analysis at a future time step using the previous time steps. Loss functions guide the model to minimize the prediction error on known data. An analysis-based verification of forecasts derived from unseen data will reveal the strength and weaknesses of the AI-WP model in reproducing the statistical and dynamical characteristics of the underlying reanalysis.

In contrast, the development and fine-tuning of traditional physics-based numerical weather prediction (NWP) systems relies on verification against observations, with the aim of reducing discrepancies relative to various observational systems. This fundamental difference raises the question of what to expect when applying observation-based verification to AI-WP models that are trained on reanalysis rather than directly on observations.

Reanalysis datasets have well-known errors with respect to observations which are documented in literature. Consequently, observation-based verification of AI-WP systems will inherently reflect the observational error characteristics of the reanalysis. Deviations from this expectation are particularly informative: a larger error than that of the reanalysis may indicate deficiencies in emulation, whereas a smaller error raises the question of whether, and from where, additional information beyond the reanalysis has been obtained.

To address these questions, we apply the multiple correlation decomposition based on partial correlations introduced by Glowienka-Hense et al. (2020). This method decomposes the explained variance of two different datasets with respect to the same observations into a component of information contained in both datasets (shared explained variance) and the respective added values, i.e., information present in one dataset but not in the other. This decomposition enables quantification of the information transferred from the reanalysis into the forecasts and reveals potential deficiencies, or improvements relative the reanalysis, in the training process. Furthermore, it facilitates comparison of different forecasting systems in terms of there shared and unique information content. The method is demonstrated using 2m-temperature station observations and global deterministic AI-WP and NWP forecasts.

Glowienka-Hense et al. (2020): Comparing forecast systems with multiple correlation decomposition based on partial correlation, ASCMO, 6, 103–113, https://doi.org/10.5194/ascmo-6-103-2020

How to cite: Wahl, S.: Observation-based verification of AI weather prediction models: What can we expect?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13910, https://doi.org/10.5194/egusphere-egu26-13910, 2026.

EGU26-14107 | Posters on site | NP5.1

Improvements to the Met Office operational Visibility diagnostic using Machine Learning  

Katharine Grant and Gavin Evans

Visibility forecasting is critical for aviation, transportation, and public safety, yet remains a challenging aspect of meteorology due to complex atmospheric processes and aerosol interactions. Accurate visibility prediction is essential for operational decision-making, but traditional approaches often struggle with physical realism and probabilistic reliability. 

This study addresses these challenges within the Met Office’s IMPROVER (Integrated Model post-PROcessing and VERification) framework, which provides probabilistic post-processing of Numerical Weather Prediction (NWP) output for customers including the UK Public Weather Service. Historically, visibility diagnostics in IMPROVER have been constrained by limitations in the underlying NWP model. To overcome this, two key enhancements were introduced. First, the integration of VERA (Visibility Employing Realistic Aerosols), an existing diagnostic within the Unified Model (UM), which incorporates polydisperse aerosol effects to deliver a more physically consistent representation of visibility.  
Second, building on this improved foundation, a statistical post-processing step was implemented using Quantile Regression Forests (QRF), marking the first application of machine learning within IMPROVER. QRF was chosen for its ability to capture complex, non-linear relationships and produce calibrated probabilistic forecasts. 

The primary objective was to improve forecast skill at operationally significant thresholds, particularly <7.5 km and <1 km, which are critical for aviation and road safety. Benchmarking on the EUPPBench dataset compared QRF against reliability calibration and Distribution Regression Networks (DRN). QRF demonstrated superior performance, achieving a 45% improvement in Ranked Probability Skill Score (RPSS) over the raw NWP output. Subsequent testing using Met Office data also showed significant improvement, with QRF delivering a 9% RPSS increase for thresholds <7.5 km and a 22% improvement in Continuous RPSS across all thresholds. 

This work demonstrates the value of combining physically realistic NWP diagnostics with machine learning techniques to enhance probabilistic visibility forecasts. These improvements pave the way for more reliable decision-making in sectors sensitive to visibility conditions. Putting this research into operational production as of early 2026 represents a significant step forward in the quality of our visibility forecasts. 

How to cite: Grant, K. and Evans, G.: Improvements to the Met Office operational Visibility diagnostic using Machine Learning , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14107, https://doi.org/10.5194/egusphere-egu26-14107, 2026.

EGU26-14658 | ECS | Posters on site | NP5.1

Representation of equatorial waves in state-of-the-art data-driven weather prediction models 

Jasmin Haupt, Hyunju Jung, Marie Müller, Steffen Tietsche, Tobias Selz, Peter Knippertz, and Julian Quinting

Equatorial waves are a key process in shaping tropical weather and have been linked to tropical-extratropical teleconnections. Besides, they are one of the reasons for the higher predictability limit in the tropics compared to the extratropics. Yet, their correct representation in weather prediction models is a long-standing challenge, even at model resolutions on the km-scale, leaving substantial potential in global weather predictions unused.

In this study, we systematically quantify and compare the representation of equatorial waves in 10-day forecasts of operational deterministic state-of-the-art weather prediction models (numerical, hybrid, and data-driven). The forecast data initialized from 01 January 2020 to 16 December 2020 are provided by WeatherBench2 and dedicated experiments with AIFS from the European Centre for Medium-Range Weather Forecasts (ECMWF). Equatorial Kelvin, Rossby, and westward-moving mixed Rossby-Gravity waves have been identified based on 850-hPa winds and geopotential height using the approach of Yang et al. (2003). The filtered data-driven forecast data are evaluated against ERA5 and operational ECMWF analysis for wave amplitude and pattern correlation, and compared with the numerical weather prediction (NWP) model Integrated Forecasting System (IFS) from ECMWF.

The key finding is that for the period 2020, all data-driven weather prediction models outperform the NWP-based forecasts of the IFS model in representing equatorial wave patterns beyond 3 days lead time, evaluated with the Pearson Correlation Coefficient, except for the Rossby wave mode n=1, which is equally well represented by all models.  
For Kelvin waves, the difference in forecast skill is most remarkable with an extension of the forecast horizon in most models from 8 to 10 days. In terms of Kelvin wave activity bias, ML-models exhibit a smaller systematic error than the IFS model, which locally underestimates the Kelvin wave activity by up to 30 % when evaluated against ERA5, with the highest underestimation in the Pacific. Interestingly, the equatorial wave representation in the data-driven model Pangu-Weather depends on the initialization dataset. We currently investigate the reason for this difference by systematically comparing ML-forecasts initialized from ERA5 and operational ECMWF analysis.

How to cite: Haupt, J., Jung, H., Müller, M., Tietsche, S., Selz, T., Knippertz, P., and Quinting, J.: Representation of equatorial waves in state-of-the-art data-driven weather prediction models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14658, https://doi.org/10.5194/egusphere-egu26-14658, 2026.

This study aims to estimate the objective amount of the supercooled liquid water content (SLWC) using in situ aircraft observation data to construct an objective and consistent long-term dataset of aircraft icing intensity. SLWC was estimated using two conventional calibration methods and a newly proposed Gated Recurrent Unit (GRU) model, based on measurements from the Rosemount Icing Detector (RICE) and collocated in situ aircraft observations. The observations were collected by NARA research aircraft operated by the National Institute of Meteorological Sciences in South Korea, which has conducted regular atmospheric observations since February 2018. The GRU-based approach demonstrated substantially improved performance compared to the calibration methods, achieving a Pearson correlation coefficient of 0.945 and a Nash–Sutcliffe efficiency of 0.891 when evaluated against independent observations not used in model training. In particular, the proposed method enables a more detailed representation of SLWC evolution by providing time-series SLWC estimates, whereas calibration-based approaches typically provide a single representative value for each icing event. The GRU-based estimates closely reproduce the observed temporal variability of SLWC in NARA icing cases, further demonstrating the capability of the proposed method to capture realistic SLWC evolution. The estimated SLWC from the proposed model were subsequently used to classify icing intensity based on operationally established SLWC thresholds for each icing intensity category, resulting in a robust long-term icing intensity dataset spanning over six years. The outcomes of this study are expected to contribute not only to aircraft icing research but also to a broad spectrum of applications including remote-sensing-based hydrometeor detection, cloud microphysical processes, and numerical weather prediction model parameterizations.

Acknowledgement: This research is supported by the Korea Meteorological Administration Research and Development Program under Grant RS-2022-KM220310 and RS-2022-KM220410.

How to cite: Kim, E.-T. and Kim, J.-H.: A Novel Method for Estimating the Supercooled Liquid Water Content Using In Situ Aircraft Observation Data and Gated Recurrent Unit, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15199, https://doi.org/10.5194/egusphere-egu26-15199, 2026.

EGU26-17204 | ECS | Orals | NP5.1

Dynamical evaluation of the error representation in the generative AI nowcasting model  LDCast 

Martin Bonte, Stéphane Vannitsem, and Lesley De Cruz

The variability in ensemble forecasts can either be generated dynamically - as is usually done with Numerical Weather Prediction (NWP) models -, stochastically or by using new approaches such as AI generative techniques. As these approaches are in their infancy for geophysical applications, the properties of the ensembles of generative models are still far from clear, especially if those models are to be used in operational activities. This aspect is investigated here for nowcasting models.

This work provides a predictability analysis over Belgium for the generative AI nowcasting model LDCast [1], as well as for the stochastic STEPS nowcasting algorithm (pysteps implementation [2]). Both models correctly estimate the error at almost all scales by means of their ensemble spread (i.e. good spread/error relationship), and they adapt the morphology of their ensembles depending on whether the event dynamics is convective or stratiform. Surrogate ensembles are also derived from the ensembles of STEPS and LDCast, and used as benchmarks with which to compare the spatial scores of the models. This reveals that both STEPS and LDCast ensembles struggle to provide added value for the spatial localization of the uncertainty associated with the growth and decay of rainfall. Therefore, STEPS and LDCast ensembles seem to be accurate statistically but not dynamically.

[1] Leinonen, J., et al. (2023). Latent diffusion models for generative precipitation nowcasting with accurate uncertainty quantification. arXiv preprint arXiv:2304.12891.

[2] Pulkkinen, S., et al. (2019). Pysteps: an open-source python library for probabilistic precipitation nowcasting (v1.0). GMD, 12(10):4185–4219.

How to cite: Bonte, M., Vannitsem, S., and De Cruz, L.: Dynamical evaluation of the error representation in the generative AI nowcasting model  LDCast, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17204, https://doi.org/10.5194/egusphere-egu26-17204, 2026.

EGU26-17479 | Orals | NP5.1

From ERA5 to Precipitation Extremes: Global km-Scale, Sub-Hourly Downscaling with Generative AI 

Luca Glawion, Julius Polz, Harald Kunstmann, Benjamin Fersch, and Christian Chwala

Global reanalysis products such as ERA5 are indispensable for climate and hydrological studies, yet their coarse spatial and temporal resolution limits the representation of localised and short-lived precipitation extremes. Building on our earlier work [1], we now present the published and ready-to-use version of spateGAN-ERA5, a generative AI framework for global spatio-temporal downscaling of ERA5 precipitation to kilometre and sub-hourly scales (2 km, 10 min) [2].

The model, trained using gauge-adjusted radar observations over Germany, generates realistic high-resolution precipitation ensembles conditioned on ERA5 inputs. We demonstrate robust performance across multiple climate regimes through independent evaluations over Germany, the United States, and Australia, showing clear improvements in spatial structure, temporal coherence, and extreme rainfall representation compared to native ERA5 fields. Ensemble generation further enables probabilistic uncertainty quantification.

To facilitate broad adoption, we provide a public, easy-to-use downscaling tool [3] that enables on-demand generation of high-resolution precipitation for any region and time period worldwide. The approach is computationally efficient and applicable on modest GPU hardware, making it suitable for both regional studies and large-scale applications. spateGAN-ERA5 thus establishes a practical pathway toward global high-resolution precipitation products for climate impact analysis, hydrological modelling, and AI-based weather and climate research.

[1] Glawion, L., Polz, J., Kunstmann, H., Fersch, B., & Chwala, C. (2023). spateGAN: Spatio‑temporal downscaling of rainfall fields using a cGAN approach. Earth and Space Science, 10, e2023EA002906. https://doi.org/10.1029/2023EA002906

[2] Glawion, L., Polz, J., Kunstmann, H., Fersch, B., & Chwala, C. (2025). Global spatio‑temporal ERA5 precipitation downscaling to km and sub‑hourly scale using generative AI. npj Climate and Atmospheric Science, 8, 219. https://doi.org/10.1038/s41612-025-01103-y

[3] https://github.com/LGlawion/spateGAN_ERA5

How to cite: Glawion, L., Polz, J., Kunstmann, H., Fersch, B., and Chwala, C.: From ERA5 to Precipitation Extremes: Global km-Scale, Sub-Hourly Downscaling with Generative AI, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17479, https://doi.org/10.5194/egusphere-egu26-17479, 2026.

EGU26-17711 | ECS | Orals | NP5.1

Probabilistic Benchmarks and Post-Processing for Data-Driven Weather Forecasting 

Tobias Biegert, Nils Koster, and Sebastian Lerch

In recent years, significant progress in machine learning technologies has enabled the development of various artificial intelligence weather prediction (AIWP) models, approaching, or even surpassing the skill of numerical weather prediction (NWP) models.

However, despite these advancements, several important questions remain open. Most data-driven models primarily focus on deterministic point forecasts and lack the capability to generate probabilistic predictions, which, however, is crucial for optimal decision making and quantifying weather risk in applications. Further, while it has been widely demonstrated that physics-based NWP models substantially benefit from post-processing methods, which aim to correct systematic errors, the use of post-processing for data-driven weather models has not been explored in detail.

Our overarching aim thus is to investigate the application of various post-processing techniques to potentially improve predictions, as well as to generate probabilistic forecasts from deterministic AIWP as well as NWP model outputs. We assess whether AI-based weather models benefit from post-processing to a similar extent as physics-based NWP, enabling a fair comparison between post-processed AIWP and NWP forecasts. The resulting post-processed AIWP forecasts also yield a relatively simple probabilistic benchmark for evaluating whether inherently probabilistic AIWP models deliver commensurate skill improvements given their increased computational cost.

Experiments are based on the WeatherBench 2 framework, which provides a standardized archive of prominent AIWP as well as operational NWP model outputs. Specifically, we apply a suite of established statistical and machine learning post-processing methods to model outputs for the eight variables defined as headline scores (Z500, T850, Q700, WV850, T2M, WS10, MSLP, TP24hr) in the WeatherBench 2 framework, and systematically evaluate the effectiveness of these methods for improving deterministic and probabilistic forecasts.

Results show that post-processed probabilistic forecasts can outperform the ensemble predictions from the European Centre for Medium-Range Weather Forecasts for shorter lead times of up to one week for selected variables, but the results vary across variables, lead times, post-processing methods and forecasting models.

How to cite: Biegert, T., Koster, N., and Lerch, S.: Probabilistic Benchmarks and Post-Processing for Data-Driven Weather Forecasting, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17711, https://doi.org/10.5194/egusphere-egu26-17711, 2026.

Taiwan is located along the circum-Pacific seismic belt and is frequently affected by destructive earthquakes. Identifying reliable preseismic anomalies is therefore crucial for seismic hazard mitigation. Previous studies have demonstrated that groundwater levels are influenced not only by nontectonic factors—such as precipitation, atmospheric pressure, tides, and temperature—but also by stress redistribution associated with earthquake preparation processes. However, robust quantitative methods capable of separating nontectonic influences from tectonic anomalies remain limited. In this study, the 2016 Meinong earthquake in southern Taiwan was investigated as a case study. Support vector regression (SVR) models were developed using meteorological variables and groundwater level observations to construct predictive models of groundwater fluctuations and to identify preseismic anomalies related to crustal stress accumulation. Groundwater monitoring stations located west of the epicenter were first selected based on their clear coseismic responses and strong spatial correspondence with observed surface deformation. Using air temperature, precipitation, and atmospheric pressure as explanatory variables, the SVR model and the Akaike Information Criterion (AIC) were applied to determine optimal lag structures and to establish pre-earthquake groundwater prediction models. The trained models were then used to simulate groundwater levels over the two years preceding the earthquake, and residual analysis was performed to identify anomalous signals. Among the 12 analyzed stations, 9 exhibited coefficients of determination (R²) ranging from 0.18 to 0.79. Stations situated in coastal fine-sand aquifers showed substantially higher predictive performance (R² = 0.42–0.79) than those located in mountainous regions (R² = 0.18–0.49). Six stations displayed pronounced negative residual anomalies exceeding two standard deviations approximately one year prior to the earthquake, followed by a gradual recovery toward the event. This temporal pattern is consistent with deformation trends observed at nearby surface monitoring stations. In addition, three stations exhibited short-term residual anomalies exceeding two standard deviations within approximately one month before the earthquake. These results demonstrate that groundwater level anomalies derived from physically informed predictive models can be systematically linked to surface deformation and short-term precursory processes preceding earthquakes. Our findings highlight the potential of groundwater monitoring as a complementary indicator for earthquake precursor detection and seismic hazard assessment.

How to cite: Mai, Y.-L., Chen, X.-N., and Lu, T.-H.: Identification of Tectonic Anomalies Prior to the Meinong Earthquake in Taiwan Using a Support Vector Regression–Based Groundwater Level Model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18581, https://doi.org/10.5194/egusphere-egu26-18581, 2026.

EGU26-18999 | Posters on site | NP5.1

Machine learning sea-surface temperature forecasting based on empirical orthogonal functions 

Takeshi Enomoto, Aki Saito, and Saori Nakashita

Data-driven forecasting of the atmosphere and ocean is evolving rapidly. Recent reports on machine learning weather prediction (MLWP) demonstrate that these models rival or even outperform traditional numerical weather prediction (NWP) from leading operational centres. While the inference is faster than physics-based models, MLWP typically requires Graphical Processing Units (GPUs) or Tensor Processing Units (TPUs) with significant memory, and the computational requirements for training remain enormous.

Certain applications prioritize efficiency, such as sea-surface temperature (SST) prediction on research vessels with limited communication bandwidth. We address this problem by proposing a light-weight alternative to convolutional neural networks (CNNs) or vision transformers (ViTs). To this end, we utilize gradient boosting, specifically XGBoost, which is highly efficient for tabular data. To incorporate spatial patterns, we conduct the Singular Value Decomposition (SVD) to derive Empirical Orthogonal Functions (EOFs). We train the model on the four years of 0.1° SST data based on Himawari over the Western Pacific (120°E–150°E, 20°N–50°N). Preliminary 5-day forecasts show a median error improvement to −0.082 K from 0.10 K and a reduction in standard deviation to 0.68 K from 0.74 K compared to the persistence baseline.

Acknowledgements: This work was supported by JSPS KAKENHI 24H02226.

How to cite: Enomoto, T., Saito, A., and Nakashita, S.: Machine learning sea-surface temperature forecasting based on empirical orthogonal functions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18999, https://doi.org/10.5194/egusphere-egu26-18999, 2026.

Uncertainty remains a major challenge in typhoon rainfall forecasting over Taiwan, even when cloud-resolving numerical weather prediction models are employed. Individual forecasts often exhibit large variability in rainfall amount and spatial distribution, particularly at long lead times, while their credibility is generally unknown at forecast time.

This study presents a machine learning–based framework for the a priori diagnosis of uncertainty in typhoon rainfall forecasts. Approximately fifteen years of cloud-resolving regional model forecasts and corresponding precipitation observations are used to quantify forecast quality through a similarity skill score (SSS), which measures the spatial agreement between forecasted and observed accumulated rainfall during the typhoon impact period. The machine learning model is designed to predict the future SSS of individual forecasts using only information available at forecast time, including diagnostics from the regional model and large-scale environmental and track-related predictors derived from global forecasts.

To ensure robust evaluation, the dataset is split by independent typhoon cases and time periods to avoid information leakage. Preliminary analyses suggest that the proposed approach can capture variations in forecast credibility, with forecasts predicted to have high SSS exhibiting a substantially higher likelihood of achieving high observed SSS.

Rather than improving rainfall forecasts themselves, this study focuses on statistical post-processing and uncertainty diagnosis, demonstrating the potential of machine learning as an objective tool for assessing the credibility of high-resolution typhoon rainfall forecasts.

How to cite: Chen, S.-H. and Wang, C.-C.: A Priori Diagnosis of Uncertainty in Cloud-Resolving Typhoon Rainfall Forecasts over Taiwan Using Machine Learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19403, https://doi.org/10.5194/egusphere-egu26-19403, 2026.

EGU26-19639 | Orals | NP5.1

Discrete Learning Algorithms for Precipitation Estimation from Commercial Microwave Links 

Guy Even, Andreas Karrenbauer, Rex Lei, Jonatan Ostrometzky, and Christian Sohler

Commercial microwave links (CMLs) are part of the infrastructure of wireless networks.  Their measured attenuations have been studied as an opportunistic source for monitoring spatiotemporal rainfall and other atmospheric phenomena. CML attenuation measurements can enhance the spatiotemporal accuracy and resolution of existing weather monitoring instruments. In addition, they serve as stand-alone weather monitoring devices in places where dedicated weather monitoring devices are scarce or do not exist.

Current techniques for 2D rainfall map reconstruction usually reduce CML measurements to virtual rain-gauges (i.e., point measurements) and rely on interpolation techniques such as inverse distance weighting or Kriging. While effective in many scenarios, these methods are suboptimal because they do not address the mis-modeling due to the reduction from a link-path attenuation integration to a single point rain-intensity measurement.

In this study, we revisit the rainfall map reconstruction problem from CML signal attenuation measurements as a principled optimization approach. We formulate the problem of the partial-to-complete field reconstruction as a physics-informed optimization problem. The reconstructed rainfall field is quantized and represented by pixel-rainfall variables whose values are constrained to agree with the observed CML signal attenuations. The resulting solution minimizes a weighted sum of the attenuation errors along the links, spatial differences between neighboring pixels, and the total rainfall in all the pixels of the map.

To evaluate our approach, we create a benchmark of hundreds of rainfall maps and CML locations and attenuations.
Rainfall maps are algorithmically extracted by identifying rain events in EURADCLIM rain maps (the European climatological high-resolution gauge-adjusted radar precipitation dataset). We identify rain events consisting of patches of about 50x50 km² over various terrain types and rain patterns.
We overlay CMLs on each patch using the free ``Four-year commercial microwave link dataset for the Netherlands'' (publicly available in the 4TU.ResearchData platfrom).
We then apply the ITU-R P.838 model at a pixel level to compute the CML attenuations based on the rainfall to obtain noiseless attenuation measurements.

We apply the inverse optimization procedure to the CML attenuations to reconstruct the rainfall maps. The accuracy of the reconstructed rainfall map is evaluated and compared with the inverse distance weighting approach.
Overall, this study reframes rainfall reconstruction from opportunistic sensing networks as a well-posed inverse problem with an explicit objective function.
Our reconstruction framework can also assist in explaining AI-solutions in the absence of ground truth.

How to cite: Even, G., Karrenbauer, A., Lei, R., Ostrometzky, J., and Sohler, C.: Discrete Learning Algorithms for Precipitation Estimation from Commercial Microwave Links, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19639, https://doi.org/10.5194/egusphere-egu26-19639, 2026.

As a proper score, the continuous ranked probability score (CRPS) is widely used within the field of statistical postprocessing of ensemble forecasts, both for forecast verification and as a loss function for parameter estimation with distributional regression approaches. This includes standard ensemble model output statistics (EMOS) and machine learning (ML) based approaches such as distributional regression networks (DRN). It is known that the CRPS admits equivalent representations as an integral of the Brier score over probability thresholds or an integral of the quantile score over quantile levels. The CRPS can be further generalized with a weighting function to put more weight on certain regions of the predictive distribution (the threshold-weighted CRPS or twCRPS), or to put more weight on certain quantiles of the distribution (quantile-weighting, denoted qwCRPS). In this work, we consider a general 2-parameter class of weight functions that give rise to an analytical expression for the qwCRPS for certain predictive distributions such as the logistic distribution. This generalized version of the CRPS puts a different penalty on over- or underforecasting the meteorological variable, allowing tailored postprocessing for end users with specific cost-loss ratios. We apply a DRN approach using the qwCRPS as loss function to various use cases, including the postprocessing of wind power forecasts for the Belgian Offshore Zone, and compare with the use of the standard CRPS as loss function. We also perform validation using the quantile score and the continuous generalisation of the relative economic value.

How to cite: Van den Bergh, J. and Smet, G.: Tailored postprocessing of ensemble forecasts with distributional regression networks and a quantile-weighted version of the continuous ranked probability score, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20150, https://doi.org/10.5194/egusphere-egu26-20150, 2026.

Weather forecasts are issued by numerical weather prediction models, which describe the dynamic behaviour of the atmosphere. Due to the chaotic nature of the atmospheric processes, assessing the uncertainty of forecasts is essential. The state-of-the-art method is to run the prediction models several times with different initialisation and/or parameterisation to obtain an ensemble of forecasts, better representing the possible scenarios.

In the last few years, AI-based models have become the centre of attention in weather forecasting due to their accuracy and efficiency. The European Centre for Medium-Range Weather Forecasts (ECMWF) has developed its Artificial Intelligence/Integrated Forecasting System (AIFS) model, which was first to provide data-driven ensemble forecasts in June 2024. Since July 2025, the AIFS ensemble model has been operational and runs in parallel with the physics-based Integrated Forecasting System (IFS) model of ECMWF, which is considered the gold standard in weather prediction. The new AIFS model can generate forecasts ten times faster than the classical physics-based one, while consuming approximately a thousand times less energy.

We present the results of our systematic comparison of the performances of the IFS and AIFS models by investigating the accuracy of raw and post-processed 10-metre wind-speed forecasts generated by the two models between July 2025 and November 2025 across several thousand station locations. The post-processed case involves the application of the parametric Ensemble Model Output Statistics method as well as a nonparametric quantile regression approach to correct any systematic biases and dispersion inaccuracies in the raw forecasts, which are usually detectable in the case of ensemble predictions.

How to cite: Kocsis, M. and Baran, S.: AI and Physics-Based Weather Forecasting: A Comparative Study of ECMWF's Operative AIFS and IFS Ensemble Wind Speed Predictions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20244, https://doi.org/10.5194/egusphere-egu26-20244, 2026.

EGU26-20598 | ECS | Posters on site | NP5.1

Efficient deep learning for radar precipitation nowcasting using spatiotemporal encoding and two-dimensional reconstruction  

Manasa Pawar, Nicoletta Noceti, and Antonella Galizia

Short-term precipitation nowcasting, the prediction of rainfall over lead times from a few minutes to about an hour, remains challenging because radar-derived precipitation fields evolve not only through motion but also through rapid, non-linear changes such as growth, decay, and structural reorganization. Classical extrapolation methods are efficient yet struggle to represent these intensity and morphology changes, while many learning-based approaches become costly when scaled to large, high-resolution radar grids. 

Our approach treats temporal learning and spatial reconstruction as two separate problems. A compact 3D convolutional encoder processes a short radar sequence to capture how precipitation structures evolve over time. We then convert the encoder feature volumes into 2D skip representations through depth aggregation and channel compression and use a lightweight 2D decoder to reconstruct full resolution forecasts. We benchmark against persistence and a strong 2D convolution baseline. 

The framework is evaluated on the RYDL dataset derived from the German Weather Service radar composite, providing 2D radar fields every five minutes over Germany at 1 × 1 km resolution on a 900 × 900 grid. Performance is benchmarked against persistence and a strong 2D convolutional baseline using complementary verification measures, including mean absolute error, critical success index at multiple intensity thresholds, and fractions skill score with spatial tolerance. Across benchmark lead times, the proposed approach reduces MAE from 0.22 to 0.20 at 5 min, from 0.35 to 0.28 at 30 min, and from 0.44 to 0.42 at 60 min relative to the 2D baseline, indicating improved robustness at intermediate horizons while retaining competitive short-range accuracy. These results suggest that combining explicit spatio-temporal encoding with efficient two-dimensional reconstruction offers a practical route to scalable radar nowcasting on large domains. 
Keywords: Radar nowcasting, precipitation forecasting, deep learning, spatio-temporal representation learning, forecast verification 

How to cite: Pawar, M., Noceti, N., and Galizia, A.: Efficient deep learning for radar precipitation nowcasting using spatiotemporal encoding and two-dimensional reconstruction , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20598, https://doi.org/10.5194/egusphere-egu26-20598, 2026.

EGU26-21878 | Orals | NP5.1

ExtremeWeatherBench 1.0: A Flexible Evaluation Framework for Extreme Weather Events 

Amy McGovern, Taylor Mandelbaum, and Daniel Rotenberg

Properly evaluating AI and NWP models before deployment will help to ensure that the final models are trustworthy. Currently, most evaluation is done at a global scale, such as with WeatherBench, rather than focusing on high-impact events. While this global evaluation is important, it can obscure the results of how a model performs on high-impact events. For example, a heat wave may be poorly forecast by one model but the model may look promising overall when examining global Root Mean Squared Error. Only by examining specific case studies do we get the bigger picture of how the model performs on phenomena that impact humanity around the world.

We introduce Extreme Weather Bench (EWB), a new community driven benchmarking suite with almost 300 case studies of high-impact weather events across the globe. EWB facilitates model validation and verification on a variety of high-impact hazards that matter to people around the globe. EWB provides a standard set of case studies (spanning multiple spatial and temporal scales and different parts of the weather spectrum), observational data, impact-based metrics, and open-source code for users to evaluate their models. The case studies include tropical cyclones, atmospheric rivers, convective weather outbreaks, heat waves and major freeze events. To facilitate ease-of-use, EWB is distributed as a pure Python package, and integrates with either local data or data saved on the cloud.

EWB will help to drive the science forward for all weather models, enabling true comparisons across models and enabling people to evaluate their models on specific high-impact phenomena while diving deeply into case studies. EWB is a free open-source community-driven system and will be adding additional phenomena, test cases and metrics in collaboration with the worldwide weather and forecast verification community.

How to cite: McGovern, A., Mandelbaum, T., and Rotenberg, D.: ExtremeWeatherBench 1.0: A Flexible Evaluation Framework for Extreme Weather Events, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21878, https://doi.org/10.5194/egusphere-egu26-21878, 2026.

EGU26-21929 | Posters on site | NP5.1

Estimation and spatial prediction methods for high-frequency space-time solar irradiance 

William Kleiber and Nicolas Coloma

As the power grid moves to a more renewable future, energy sources from weather-driven phenomena such as solar power will form an increasingly large portion of electricity generation.  The predicatibility, non-Gaussianity and intermittency of solar resources challenge current grid operation paradigms, and realistic data scenarios are required for grid planning and operational studies.  However, such data are not available at the space-time resolution needed for realistic grid models.  Given sparse spatial samples that are high-resolution in time, we introduce a framework for spatiotemporal prediction and downscaling in a functional data analysis framework when data exhibit nonstationary phase misalignment.  The approach is illustrated on a challenging irradiance dataset and compares favorably against existing methods.

How to cite: Kleiber, W. and Coloma, N.: Estimation and spatial prediction methods for high-frequency space-time solar irradiance, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21929, https://doi.org/10.5194/egusphere-egu26-21929, 2026.

EGU26-719 | ECS | Posters on site | AS5.1

Does AI Learn Physics? Assessing the Physical Fidelity of Data-Driven Tropical Cyclone Forecasts 

Pankaj Sahu, Sukumaran Sandeep, and Hariprasad Kodamana

Machine Learning Weather Prediction (MLWP) models—specifically GraphCast, PanguWeather, Aurora, and FourCastNet—show great promise for competing with physics-based Numerical Weather Prediction (NWP) models by providing global forecasts at a low computational cost. However, a thorough physical evaluation is needed before they can be used in place of NWP models. Our comprehensive study comparing these four leading MLWP models with NWP and observations in Tropical Cyclone (TC) forecasting across all tropical basins uncovers a significant duality: MLWP models are very good at predicting the TC track (with an average error of less than 200 km at a 96-hour lead time) because they accurately capture the underlying dynamics. However, they always underestimate the maximum sustained wind speeds (intensity). This systematic low intensity bias is directly related to biases that come from their ERA5 training data and are made worse by penalties. Even with this limitation, the models accurately depict important physical structures, such as low-level convergence and the vertical warm core, while also keeping different physical fields consistent. This suggests that the models learn how different dynamical and thermodynamical processes are related to each other in a way that makes sense. Ultimately, although MLWPs, especially Aurora, exhibit an implicit comprehension of TC dynamics, their enduring intensity bias requires additional refinement prior to their complete substitution of NWP models.

How to cite: Sahu, P., Sandeep, S., and Kodamana, H.: Does AI Learn Physics? Assessing the Physical Fidelity of Data-Driven Tropical Cyclone Forecasts, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-719, https://doi.org/10.5194/egusphere-egu26-719, 2026.

EGU26-2452 | ECS | Posters on site | AS5.1

Climate Grey-Box Flow Matching for Robust Climate and Weather Prediction 

Gurjeet Singh, Frantzeska Lavda, and Alexandros Kalousis
Deep generative models such as flow matching and diffusion models have great potential for learning complex dynamical systems, but they typically act as black boxes, neglecting underlying physical structure. In contrast, physics-based models governed by ODEs and PDEs provide interpretability and physical consistency, yet are often incomplete due to unresolved processes, missing source terms, or uncertain parameterisations. Bridging these two paradigms is a central challenge in data-driven weather and climate modelling.

We propose a Climate Grey-Box Dynamics Matching framework designed for weather and climate systems, that explicitly combines existing physical models with data-driven learning to capture unresolved dynamics where known physical operators are directly embedded into the learned dynamics. Our framework learns from observational trajectories alone and operates in a simulation-free manner inspired by gradient matching and flow matching methods. By avoiding numerical solvers, it eliminates the memory overhead, computational cost, and numerical instability associated with Neural ODE–based approaches.

To capture temporal dependencies in our simulation-free method, we introduce a lightweight attention-based temporal encoder that aggregates short-term history in a physically consistent manner. This design enables the model to represent unresolved dynamics without increasing computational complexity, making it well-suited for high-dimensional spatiotemporal climate systems. We apply this framework to weather and climate forecasting and demonstrate its effectiveness against ClimODE, a state-of-the-art solver-based grey-box model. Reformulating ClimODE as a simulation-free grey-box model reduces training complexity from Ο(L) to Ο(1), where L denotes the number of solver steps. Beyond computational gains, the simulation-free formulation yields substantial memory efficiency: training is possible on a single RTX 3060 (12 GB), whereas ClimODE requires at least 25 GB of GPU memory with a small batch size. This enables efficient training on commodity hardware and improves accessibility for large-scale climate modelling.

Experiments on weather and climate benchmarks show that the proposed method achieves improved forecast accuracy and faster convergence compared to simulation-based and fully data-driven baselines. The method demonstrates particular robustness to long horizons, as performance gains become more pronounced with extended forecast times—indicating enhanced temporal stability and resistance to error accumulation, an essential property for reliable long-range climate prediction.

How to cite: Singh, G., Lavda, F., and Kalousis, A.: Climate Grey-Box Flow Matching for Robust Climate and Weather Prediction, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2452, https://doi.org/10.5194/egusphere-egu26-2452, 2026.

Artificial intelligence (AI)-based data-driven weather prediction (AIWP) models have experienced rapid progress over the last years. They achieve impressive results and demonstrate substantial improvements over state-of-the-art physics-based numerical weather prediction (NWP) models across a range of variables and evaluation metrics. However, most efforts in data-driven weather forecasting have been limited to deterministic, point-valued predictions, making it impossible to quantify forecast uncertainties, which is crucial in research and for optimal decision making in applications.

I will present recent work on uncertainty quantification (UQ) methods in the context of data-driven weather prediction. The post-hoc use of UQ methods enables the generation of skillful probabilistic weather forecasts from a state-of-the-art deterministic AIWP model [1]. Further, by subjecting the deterministic backbone of physics-based and data-driven models post hoc to the same UQ technique, and computing the in-sample mean continuous ranked probability score of the resulting forecast, we propose a new measure that enables fair and meaningful comparisons of single-valued output from AIWP and NWP models, called potential continuous ranked probability score [2].

References

[1] Bülte, C., Horat, N., Quinting, J. and Lerch, S. (2025). Uncertainty quantification for data-driven weather models. Artificial Intelligence for the Earth System, in press. DOI:10.1175/AIES-D-24-0049.1

[2] Gneiting, T., Biegert, T., Kraus, K., Walz, E.-M., Jordan, A. I., and Lerch, S. (2025). Probabilistic measures afford fair comparisons of AIWP and NWP model output. Preprint, arXiv:2506.03744. DOI:10.48550/arXiv.2506.03744

How to cite: Lerch, S.: Uncertainty quantification for data-driven weather prediction: From probabilistic forecasts to fair model comparisons, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2971, https://doi.org/10.5194/egusphere-egu26-2971, 2026.

EGU26-3091 | ECS | Posters on site | AS5.1

Learning to sample unprecedented atmospheric rivers 

Tim Whittaker and Alejandro Di Luca

Atmospheric rivers (ARs) are the dominant drivers of hydrological extremes along the western coast of North America, yet the physical upper limits of their intensity remain poorly understood and weakly constrained by the short observational record. While thermodynamic amplification of ARs under climate change is well-documented, the potential for dynamical amplification driven by the wind field remains uncertain and computationally expensive to sample using conventional techniques such as large ensembles of simulations. Here, we address this sampling barrier by leveraging techniques from machine learning, specifically combining a differentiable global climate model with high-resolution regional downscaling to generate storylines of unprecedented AR events in western Canada. By formulating the event generation as an optimal control problem, we compute the gradients of the model’s output to learn minimal, physically plausible perturbations to historical initial states that maximize AR’s associated integrated vapour transport at landfall. These optimized storylines are further dynamically downscaled using a high-resolution regional climate model, producing extreme precipitation events that significantly exceed historical benchmarks. 

How to cite: Whittaker, T. and Di Luca, A.: Learning to sample unprecedented atmospheric rivers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3091, https://doi.org/10.5194/egusphere-egu26-3091, 2026.

EGU26-3927 | Posters on site | AS5.1

Few-shot learning for mid-latitude climate forecasts 

Yoo-Geun Ham, Seol-Hee Oh, and Gyuhui Kwon

Reliable prediction of climate variables and high-impact extremes in the midlatitudes is crucial for climate risk assessment, agricultural planning, water resource management, and disaster preparedness. However, conventional deep learning–based approaches for midlatitude climate prediction trained with dynamical climate models (e.g., CMIP models) can cause systematic errors in capturing the observed climate-relevant signals, ultimately limiting prediction skill. These limitations highlight the need to improve midlatitude prediction by detecting climate signals solely from the limited numbers of reliable observational climate data. To address the challenge of limited training samples, we employ the model-agnostic meta-learning (MAML) algorithm along with domain-knowledge-based data augmentation to predict mid-latitude winter temperatures. The proposed data augmentation is purely based on the observed data by defining the labels using large-scale climate variabilities associated with the target variable. The MAML-applied convolutional neural network (CNN) demonstrates superior correlation skills for winter temperature anomalies compared to a reference model (i.e., the CNN without MAML) and state-of-the-art dynamical forecast models across all target lead months during the boreal winter seasons. Moreover, occlusion sensitivity results reveal that the MAML model better captures the physical precursors that influence mid-latitude winter temperatures, resulting in more accurate predictions.

How to cite: Ham, Y.-G., Oh, S.-H., and Kwon, G.: Few-shot learning for mid-latitude climate forecasts, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3927, https://doi.org/10.5194/egusphere-egu26-3927, 2026.

EGU26-4301 * | Orals | AS5.1 | Highlight

Numerical models outperform AI weather forecasts of record-breaking extremes 

Zhongwei Zhang, Erich Fischer, Jakob Zscheischler, and Sebastian Engelke

Artificial intelligence (AI)-based models are revolutionizing weather forecasting and have surpassed leading numerical weather prediction systems on various benchmark tasks. However, their ability to extrapolate and reliably forecast unprecedented extreme events remains unclear. Here, we show that for record-breaking weather extremes, the numerical model High RESolution forecast (HRES) from the European Centre for Medium-Range Weather Forecasts still consistently outperforms state-of-the-art AI models GraphCast, GraphCast operational, Pangu-Weather, Pangu-Weather operational, and Fuxi. We demonstrate that forecast errors in AI models are consistently larger for record-breaking heat, cold, and wind than in HRES across nearly all lead times. We further find that the examined AI models tend to underestimate both the frequency and intensity of record-breaking events, and they underpredict hot records and overestimate cold records with growing errors for larger record exceedance. Our findings underscore the current limitations of AI weather models in extrapolating beyond their training domain and in forecasting the potentially most impactful record-breaking weather events that are particularly frequent in a rapidly warming climate. Further rigorous verification and model development is needed before these models can be solely relied upon for high-stakes applications such as early warning systems and disaster management.

How to cite: Zhang, Z., Fischer, E., Zscheischler, J., and Engelke, S.: Numerical models outperform AI weather forecasts of record-breaking extremes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4301, https://doi.org/10.5194/egusphere-egu26-4301, 2026.

EGU26-5719 | ECS | Posters on site | AS5.1

An AI-based framework for high-resolution climate dataset over Italy: from historical reconstruction to an operational chain 

Ilenia Manco, Otavio Medeiros Feitosa, Mario Raffa, and Paola Mercogliano

High-resolution climate datasets are fundamental for monitoring extreme events, assessing climate variability, and supporting climate adaptation strategies. However, producing high-resolution climate reanalyses usually requires computationally expensive dynamical downscaling. As a result, near–real-time high-resolution climate services remain limited, since most downscaling products are generated retrospectively with delays of months to years (Hersbach et al., 2020; Harris et al., 2022). Recent advances in generative machine learning enable realistic fine-scale atmospheric fields that preserve spatial coherence and key statistics, including extremes (Rampal et al., 2025; Camps-Valls et al., 2025). Hybrid statistical–dynamical approaches therefore provide an efficient and physically consistent pathway for operational high-resolution dataset production (Glawion et al., 2025; Schmidt et al., 2025). This work presents the progress achieved in the development of a high-resolution climate datasets over the Italian Peninsula at 2.2 km resolution, exploiting a conditional Generative Adversarial Network (cGAN) model developed in Manco et al. (2025). The framework follows a hybrid statistical–dynamical downscaling strategy, in which ERA5 reanalysis data at 0.25° resolution are downscaled using cGANs trained against the very-high-resolution dynamical product VHR-REA_IT (Raffa et al., 2021). The system has been extended to multiple near-surface atmospheric variables, including mean, minimum, and maximum 2 m temperature, relative surface humidity, cumulative precipitation, and 10 m wind (speed and direction), the latter two representing particularly challenging targets (Fig. 1). Each variable is downscaled using a dedicated cGAN trained independently to learn the non-linear spatial relationships between coarse-resolution ERA5 predictors and high-resolution VHR-REA_IT targets, while employing a common network architecture and loss function to ensure methodological consistency. This enabled the production of a high-resolution historical dataset covering the period 1990–2024 at daily frequency, with 1990–2000 used for training. Since January 2025, the framework (Fig. 2) has been integrated into an operational chain and used to generate high-resolution fields in near real time, automatically updating the dataset as new ERA5 data become available, with an average latency of approximately six days. All data are distributed in NetCDF format through the CMCC Data Delivery System (https://dds.cmcc.it/) within the FAIR (Fast AI Reanalysis) product, with daily maps accessible via the Dataclime dashboard (https://www.dataclime.com/). Both deterministic and probabilistic configurations of the cGAN framework are presented. Results, evaluated against the dynamically downscaled fields available at the same resolution over the common historical period, show that the proposed approach robustly reproduces spatial patterns (Fig. 3), mean values, and variability across all variables. The probabilistic configuration improves uncertainty representation and shows skill in capturing both mean conditions and extremes. Overall, the framework represents a versatile and robust solution for the generation of high-resolution climate datasets in both historical and operational contexts. Remaining limitations primarily concern the representation of extreme precipitation percentiles in regions characterized by complex orography, which will be the focus of future developments.

Fig. 1 – Wind speed at 10 m for a random day.

Fig. 2 - c-GAN Training Framework

Fig. 3 – Seasonal Analysis. 2-m minimum temperature.

 

How to cite: Manco, I., Feitosa, O. M., Raffa, M., and Mercogliano, P.: An AI-based framework for high-resolution climate dataset over Italy: from historical reconstruction to an operational chain, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5719, https://doi.org/10.5194/egusphere-egu26-5719, 2026.

EGU26-6394 | ECS | Orals | AS5.1

A review of spatially explicit climate emulators for enhancing modelling agility 

Sarah Schöngart, Lukas Gudmunsson, Chris Womack, Carl-Friedrich Schleussner, and Sonia Seneviratne

Machine-learning-based weather and climate emulators are rapidly transforming how climate information is generated and applied by enabling fast scenario exploration, large ensemble analysis, and the generation of decision-relevant climate data at scales beyond the reach of traditional climate models. Emulators are increasingly integrated into policy-relevant assessments and are expected to play a growing role in upcoming IPCC reports. Yet the field remains fragmented as task definitions and evaluation standards differ across communities, and frameworks for connecting short-term weather emulation to long-term climate projections are missing..

Here, we synthesise 77 studies on spatially explicit climate, hybrid weather-climate, and weather emulators within a unified conceptual framework, mapping inputs and outputs, methodological choices, validation practices, and computational requirements. Three structural patterns emerge. First, most climate emulators prioritise computational speed and scenario agility but offer limited output flexibility, typically generating gridded fields for a narrow set of variables. Second, the emulator landscape is fragmented: weather and hybrid weather-climate emulators form a coherent, machine-learning-driven cluster, whereas climate emulators are more heterogeneous, less connected to machine-learning advances, and validated inconsistently. Third, state-of-the-art weather emulators often rely on specialised hardware and institutional resources concentrated in a few organisations, raising questions of computational equity and “agility for whom”.

Our findings suggest that realizing genuine agility will require future research to focus on user-tailored outputs, rigorous evaluation across forcing scenarios, cross-domain methodological integration, and equitable access to computational resources. These priorities will help the field transition from methodological innovation toward policy-relevant application.

How to cite: Schöngart, S., Gudmunsson, L., Womack, C., Schleussner, C.-F., and Seneviratne, S.: A review of spatially explicit climate emulators for enhancing modelling agility, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6394, https://doi.org/10.5194/egusphere-egu26-6394, 2026.

EGU26-7801 | Posters on site | AS5.1

Bridging Physics and Machine Learning to Enhance Weather Forecasting at ECCC 

Emilia Diaconescu, Jean-François Caron, Valentin Dallerit, Stéphane Gaudreault, Syed Husain, Shoyon Panday, Carlos Pereira Frontado, Leo Separovic, Christopher Subich, Siqi Wei, and Sasa Zhang

Environment and Climate Change Canada (ECCC) is actively advancing the integration of artificial intelligence (AI) into numerical weather prediction (NWP) through a coordinated research-to-operations strategy that combines state-of-the-art machine learning approaches with established physical modeling frameworks. This presentation summarizes the progress achieved to date.

We first describe the development of GEML (Global Environmental eMuLator), a global AI forecast model, based on Google DeepMind’s GraphCast, trained and fine-tuned in-house using ERA5 reanalysis and ECMWF operational analyses. Building on GEML, ECCC has implemented an experimental hybrid AI–NWP global forecasting system, GDPS-SN, which applies large-scale spectral nudging to improve the operational Global Deterministic Prediction System (GDPS) by leveraging the large-scale accuracy of GEML.

The presentation also introduces a description of PARADIS, a fully Canadian, physically inspired, AI-based weather forecast model, developed by ECCC and its partners. These activities illustrate ECCC’s strategic vision for AI-enabled weather prediction by combining scientific rigor, collaboration and  operational relevance to deliver more accurate forecasting systems.

 

How to cite: Diaconescu, E., Caron, J.-F., Dallerit, V., Gaudreault, S., Husain, S., Panday, S., Pereira Frontado, C., Separovic, L., Subich, C., Wei, S., and Zhang, S.: Bridging Physics and Machine Learning to Enhance Weather Forecasting at ECCC, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7801, https://doi.org/10.5194/egusphere-egu26-7801, 2026.

EGU26-8656 | Posters on site | AS5.1

Harnessing Data-Driven Weather Prediction (DWP) Model for Climate Modeling 

Chia-Ying Tu, Yu-Chi Wang, Chung-Cheh Chou, and Zheng-Yu Yan

Recent advancements in AI/ML-based Data-Driven Weather Prediction (DWP) have revolutionized meteorological forecasting. By leveraging deep learning architectures trained on the ECMWF ERA5 reanalysis, DWP models can iteratively predict atmospheric states with accuracy comparable to traditional Numerical Weather Prediction (NWP) while requiring orders of magnitude less computational power. However, DWP’s reliance on historical training data poses challenges for climate-scale simulations, particularly in representing evolving phenomena influenced by non-stationary climate change. This study investigates the applicability of the GraphCast DWP model for climate research, specifically focusing on its potential for global climate downscaling and bias correction.

To evaluate performance across varying initial conditions, we conducted three distinct 72-hour GraphCast integration experiments. The first experiment utilized high-resolution (0.25°) ERA5 data from 2000–2010 to assess model reproducibility (H-ERA5), while the second experiment employed low-resolution (1.0°) ERA5 data to quantify sensitivity to initial horizontal grid spacing (L-ERA5). In the third experiment, we utilized 36 years (1979–2014) of HiRAM climate simulations as initial conditions to evaluate a novel DWP-based climate modeling framework (GC-HiRAM).

Results from the H-ERA5 and L-ERA5 experiments demonstrate that GraphCast effectively reproduces the climate mean state and variance of the ERA5 dataset. However, both experiments exhibited an underestimation of tropical cyclone (TC) frequency and intensity, consistent with known TC climatology biases in ERA5. Notably, the GC-HiRAM experiment closely aligned with the mean states and long-term trends of the original HiRAM simulations while yielding precipitation and surface temperature variances comparable to ERA5. Interestingly, the inherent TC underestimation in GraphCast served as a functional bias correction for HiRAM, which traditionally overestimates TC frequency, thereby improving overall simulation skill. Our findings suggest that this innovative DWP-driven approach provides a computationally efficient and robust framework for global climate modeling, effectively capturing essential climate phenomena while introducing a viable pathway for high-resolution climate downscaling and ensemble simulations.

How to cite: Tu, C.-Y., Wang, Y.-C., Chou, C.-C., and Yan, Z.-Y.: Harnessing Data-Driven Weather Prediction (DWP) Model for Climate Modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8656, https://doi.org/10.5194/egusphere-egu26-8656, 2026.

Recently developed AI weather models have been widely recognized for revolutionizing weather prediction, producing forecasts more skillful than traditional models at a fraction of the computational cost. Here I will argue that the next phase of the revolution involves the adjoints of these models, applied to a wide range of problems, including novel exploration of dynamical process in weather and climate variability, extreme events, and new data assimilation systems. Adjoints are derived from gradient operations on the forward model, and are useful for measuring the sensitivity of model outputs to inputs and parameters. Historically adjoints have been derived for a limited set of traditional models, and mainly applied to problems in data assimilation. The ubiquitous availability of adjoints for AI models makes these tools easily accessible and available for a much wider range of applications. Specific examples I will discuss include shadowing trajectories for predictability, "gray swans" and a factory for out-of-sample extreme events, and mechanistic interpretability of specific phenomena.

How to cite: Hakim, G.: Using Adjoints of AI-based Weather Models to Study Predictability and Extreme Events, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8870, https://doi.org/10.5194/egusphere-egu26-8870, 2026.

EGU26-9387 | Orals | AS5.1

Evaluating emergent climate behaviour in a hybrid machine learned atmosphere -- dynamical ocean model 

Hannah Christensen, Bobby Antonio, and Kristian Strommen

Understanding how fast atmospheric variability shapes slow climate variability and sensitivity is a central challenge in Earth-system science. Recent advances in machine-learned (ML) atmospheric models have demonstrated remarkable skill on weather timescales, but their emergent behaviour in a fully coupled climate system is largely unexplored. We present results from a new hybrid modelling framework that couples a machine-learned atmosphere to a dynamical ocean model. We report on a set of 70-year coupled simulations (1950–2020 historical forcing and fixed-1950s control) in which the ACE2 ML climate emulator is interactively coupled to the NEMO ocean model. These experiments represent, to our knowledge, the first multi-decadal integrations of a machine-learned atmosphere interacting with a full-depth dynamical ocean. We assess the behaviour of the coupled system, with particular focus on low-frequency tropical variability and the climate response to greenhouse-gas forcing. Preliminary results indicate realistic emergent El Nino-like variability and a physically plausible climate sensitivity, suggesting that key atmosphere–ocean feedbacks can be captured within a hybrid ML–dynamical framework. These results evaluate the possible role of entirely machine-learned components in next-generation Earth-system models.

How to cite: Christensen, H., Antonio, B., and Strommen, K.: Evaluating emergent climate behaviour in a hybrid machine learned atmosphere -- dynamical ocean model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9387, https://doi.org/10.5194/egusphere-egu26-9387, 2026.

EGU26-9811 | ECS | Posters on site | AS5.1

Explaining neural networks for detection of atmospheric features in gridded data 

Tim Radke, Susanne Fuchs, Iuliia Polkova, Christian Wilms, Johanna Baehr, and Marc Rautenhaus

Detection of atmospheric features in gridded datasets is typically done by means of rule-based algorithms. Recently, the feasibility of learning feature detection tasks using supervised learning with convolutional neural networks (CNNs) has been demonstrated. This approach corresponds to semantic segmentation tasks widely investigated in computer vision. However, while in recent studies the performance of CNNs was shown to be comparable to human experts, CNNs are largely treated as a “black box”, and it remains unclear whether they learn the features for physically plausible reasons. Here, we build on recently published studies that discuss datasets containing features of tropical cyclones (TCs), atmospheric rivers (ARs), and atmospheric surface fronts (SFs) as detected by human experts. We adapt the explainable artificial intelligence technique “Layer-wise Relevance Propagation” to the semantic segmentation task and investigate which input information CNNs with the Context-Guided Network (CGNet) and U-Net architectures use for feature detection. We find that for the detection of TCs and ARs, both CNNs indeed consider plausible patterns in the input fields of atmospheric variables. For instance, relevant patterns include point-shaped extrema in vertically integrated precipitable water (TMQ) and circular wind motion for TCs. For ARs, relevant patterns include elongated bands of high TMQ and eastward winds. Such results help to build trust in the CNN approach. In contrast, for the detection of SFs, we find only partially physically plausible patterns. While U-Net uses regions of changing temperature and humidity as well as strong wind shears to detect SFs, we also find noisy patterns relating to spurious correlations with the background data. To assess whether these implausible patterns reduce U-Net's generalizability, we evaluate it on a different SF dataset. Here, depending on the domain, SFs are often erroneously detected, especially in the Tropics and Arctic, highlighting the importance of analyzing whether patterns learned by a CNN are physically plausible. We also demonstrate application of the approach for finding the most relevant input variables and evaluating detection robustness when changing the input domain.

How to cite: Radke, T., Fuchs, S., Polkova, I., Wilms, C., Baehr, J., and Rautenhaus, M.: Explaining neural networks for detection of atmospheric features in gridded data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9811, https://doi.org/10.5194/egusphere-egu26-9811, 2026.

EGU26-12464 | Posters on site | AS5.1

Attribution of convective rainfall events using AI-downscaling – how extreme can we go? 

Georgie Logan, Daniel Cotterill, Mark McCarthy, Andrew Ciavarella, Henry Addison, Peter Watson, and Tomas Wetherell

Probabilistic attribution of extreme events requires large-ensemble climate model simulations, for both present and counterfactual climates, to adequately capture the tails of the distribution. Accurately modelling rainfall extremes, particularly those involving convection, or rainfall over regions with complex topography, requires high-resolution climate models. High-resolution climate data is particularly important for impact attribution to simulate realistic flood inundation as input to flood models.

Large ensembles of climate model runs for pre-industrial climates do not currently exist at convection-permitting resolution, as conventional convection-permitting models are computationally expensive to run. Therefore, attribution studies on extreme localised convective rainfall events are limited, despite the large impacts these events have on society.

To address this, we create a convective-permitting-resolution, large-ensemble dataset for England and Wales using a generative AI approach to downscale a pre-existing large ensemble of attribution runs from the HadGEM3 climate model. We use the diffusion model CPMGEM from Addison et al. (2025), which is trained and tested on the convection-permitting-resolution UK local Climate Projections data. We use CPMGEM, which enables stochastic generation of multiple samples per coarse model input, to generate multiple high-resolution precipitation samples from our original large-ensemble dataset. This process is relatively computationally cheap and enables creation of a high-resolution dataset that is larger than the input dataset.

We first investigate the ability of CPMGEM to be applied to a different configuration of the model it was trained on, and on an alternative set of counterfactuals. We also explore its ability to conserve climate trends and reproduce realistic values for the extremes.

We then assess the validity of using the downscaled dataset for attribution studies. If suitable, we will revisit a number of relevant attribution studies of extreme rainfall events and compare the original results from the coarse climate model HadGEM3-A to our new results using the high-resolution downscaled CPMGEM output. Overall, this could significantly extend the capability to attribute localised extreme rainfall events.

How to cite: Logan, G., Cotterill, D., McCarthy, M., Ciavarella, A., Addison, H., Watson, P., and Wetherell, T.: Attribution of convective rainfall events using AI-downscaling – how extreme can we go?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12464, https://doi.org/10.5194/egusphere-egu26-12464, 2026.

EGU26-13814 | ECS | Posters on site | AS5.1

Statistical Calibration of ArchesWeatherGen for Enhanced Sub-Seasonal and Longer Predictions 

Robert Brunstein and Christian Lessig

The capabilities and skill of emerging data-driven weather forecasting and climate models are steadily increasing and significant progress has been made in terms of their quality in the last years. Data-driven weather forecasting models predict the state of the atmosphere for a single step, e.g. 6h. Longer lead times are obtained using time-stepping where predictions are fed back into the model for the next step. Although many models exhibit stable behaviour for long rollouts, the training only considers short trajectories. The trained models are therefore statistically not well calibrated at longer lead times and for phenomena like blocking patterns or teleconnections, which happen on time scales larger than a few days, the predictions are poorly constrained by the training. To address this issue, the training of data-driven models needs to consider information about the atmospheric conditions from several days up to several weeks. 

We approach this problem by using ArchesWeather and ArchesWeatherGen. ArchesWeather provides a deterministic prediction of the next state of the atmosphere. ArchesWeatherGen, a probabilistic flow-matching model, corrects  the deterministic prediction to obtain a probabilistic prediction that matches the ground truth state. We tackle the long lead time calibration problem by applying ArchesWeatherGen after a large number of deterministic forecasting steps, in contrast to the single step used for ArchesWeatherGen for medium-range weather forecasting. We therefore condition ArchesWeatherGen on an entire long forecast trajectory produced by the deterministic model. Through this, ArchesWeatherGen obtains more temporal information about the atmosphere as well as the error development and can explicitly learn longer-time correlation patterns in the atmospheric dynamics. This leads to a better calibrated model at longer lead times. It also reduces the number of diffusion steps, and hence the computational costs, as we only correct the mean prediction after a larger number of deterministic autoregressive forecasting steps. For our study, we examine the influence of the length of the input trajectory and evaluate the improvement of our approach compared to the results obtained with a single step model correction.

How to cite: Brunstein, R. and Lessig, C.: Statistical Calibration of ArchesWeatherGen for Enhanced Sub-Seasonal and Longer Predictions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13814, https://doi.org/10.5194/egusphere-egu26-13814, 2026.

EGU26-15037 | ECS | Orals | AS5.1

Evaluating ArchesWeather and ArchesWeatherGen under Multi-Decadal AMIP-style climate simulations 

Renu Singh, Robert Brunstein, Antonia Anna Jost, Yana Hasson, Guillaume Couairon, Christian Lessig, and Claire Monteleoni

The last 5 years have seen an AI revolution in weather forecasting with data-driven models trained on ERA5 (such as Pangu-Weather, GraphCast) surpassing the skill of numerical models at a fraction of the compute costs . Furthermore, stochastic modeling approaches are now state-of-the-art as they can model the uncertainty in the dynamics of the earth system (GenCast, FGN). Similarly, there have been recent advances in long-term climate emulation using data-driven methods, although they either use deterministic models (ACE2, Lucie) or are trained on simulated climate data from physical models (ArchesClimate). Here, we evaluate a stochastic modeling approach, ArchesWeatherGen, on historical climate timescales (last 40 years) and its response to ocean forcings in an AMIP run setup (atmospheric model forced with sea surface temperature and sea ice). These simulations contribute to AIMIP (AI Model Intercomparison Project), an initiative to organize and compare the current state-of-the-art AI climate models. 

ArchesWeather and ArchesWeatherGen are efficient data-driven models built for medium-range weather forecasting. ArchesWeather is a deterministic transformer-based model and ArchesWeatherGen is a probabilistic generative model based on flow matching, with the same transformer backbone, that corrects the deterministic model prediction and accounts for variability in the time evolution.

In adherence to the AIMIP Stage 1 protocol, we adapt the models to serve as an atmospheric climate model for AMIP climate simulations on the historical period of 1979-2024. ArchesWeather and ArchesWeatherGen are extended to take into account monthly mean forcings for sea surface temperature (SST) and sea ice cover computed from ERA5. These models are trained on daily averaged 1-degree ERA5 data and they predict the state of the atmosphere at a forecast lead time of 24 hours given initial conditions.

We examine the ability of both models to stably emulate the current climate by quantitatively and qualitatively comparing them to the ERA5 climatology. Our results show that the models are able to emulate the current climate faithfully and reproduce many teleconnections as well as modes of annular variability correctly. We ablate different model configurations against each other and investigate the influence of the residual predictions of ArchesWeatherGen on the quality of the climate simulations compared to the deterministic predictions of ArchesWeather. We also analyse the models' capability to reproduce extreme weather statistics. Lastly, we examine the models’ response to forcings by evaluating the stability, trend, and physical correlations when running the model in different forcing scenarios, such as no forcings, annually repeating forcings, and increased SST.

How to cite: Singh, R., Brunstein, R., Jost, A. A., Hasson, Y., Couairon, G., Lessig, C., and Monteleoni, C.: Evaluating ArchesWeather and ArchesWeatherGen under Multi-Decadal AMIP-style climate simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15037, https://doi.org/10.5194/egusphere-egu26-15037, 2026.

EGU26-15189 | ECS | Posters on site | AS5.1

How can AI tools be used to explore unprecedented future climate and weather extremes? 

Tom Wood and Tom Matthews

This study addresses recent calls for greater focus on understanding unprecedented extreme events (e.g. Kelder et al., 2025; Matthews et al., in review) by exploring the potential to use downscaled ‘synthetic data’ from climate model projections to train cutting-edge, computationally efficient deep learning models and generate very large ensembles of high-resolution extreme weather events under future perturbed climates. The study seeks to advance understanding of plausible upper limits in extreme high-impact, low-likelihood (HILL), record-shattering extremes and unprecedented tail risks, focusing initially on the threat of uncompensable heat with the potential to result in catastrophic mass mortality impacts. We address a number of open questions in this nascent field by testing a set of recently developed tools in new and innovative ways to understand the benefits and limitations of this approach. 

Can we generate new insights beyond what can be achieved using traditional methods, such as large ensembles of physics-based models and advances such as ensemble boosting? What are the benefits of producing very large stochastic ensembles of plausible extreme weather systems and how does this complement (or otherwise) other approaches with similar motivations (e.g. emulators)? Can we identify and validate plausible physical climate storylines leading to unprecedented extreme events e.g., by identifying and clustering meteorological setups leading to very large, compound, or concurrent non-contiguous regional extremes? Can we robustly constrain this method to ensure physical plausibility in unprecedented climates? Can we advance understanding of rare event probability under a non-stationary climate from various emissions pathways? What are the limitations due to aleatoric and epistemic uncertainty? How do we mitigate biases and limit their propagation? Can we investigate downward counterfactuals and identify meteorological conditions aligning with imagined worst-case scenarios?

By addressing these questions, this study seeks to advance knowledge of the threats posed by the most extreme plausible weather events posing potentially catastrophic risks to society.

How to cite: Wood, T. and Matthews, T.: How can AI tools be used to explore unprecedented future climate and weather extremes?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15189, https://doi.org/10.5194/egusphere-egu26-15189, 2026.

The Western North Pacific Subtropical High (WNPSH) is one of the dominant subtropical anticyclonic circulations over the western North Pacific during boreal summer, strongly influencing East Asian extremes such as tropical cyclone tracks, heatwaves, and the Baiu/Meiyu front. WNPSH variability reflects both midlatitude teleconnections and tropical intraseasonal oscillations (BSISO). Therefore, to clarify predictability, it is essential to identify and quantify how individual events contribute to forecast skill and uncertainty.

We develop a probabilistic deep learning framework to predict a WNPSH index with explicit uncertainty, represented as Gaussian regression outputs (μ, σ), and assess its predictability up to a 1-month lead. We adopt a model that combines a three-dimensional convolutional neural network with self-attention. To capture diverse representations, we pretrain the model using a millennial-scale ensemble dataset from d4PDF and then fine-tune it with the ERA5 reanalysis. As a result, the prediction skill reaches ACC = 0.6 at 10-day lead time. With deep learning models, the prediction problem can be formulated as an explainable AI (XAI) task, in which precursor signals relevant to the forecast can be estimated directly from spatial patterns and input variables (Maeda and Satoh, 2025). Here, we analyze the predictability using a combination of XAI and the concept of windows of opportunity. During opportunity events, forecast skill improves to about a 15-day lead time. Clear precursor patterns emerge in the initial conditions, including signatures of intraseasonal oscillations and midlatitude wave trains. These signals are consistent with heatmap-based interpretations from XAI, providing quantitative statistics on the sources of predictability for prominent events.

How to cite: Maeda, Y. and Satoh, M.: Probabilistic Deep Learning Identifies Windows of Opportunity and Precursors for Western North Pacific Subtropical High Prediction, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16518, https://doi.org/10.5194/egusphere-egu26-16518, 2026.

EGU26-16579 | ECS | Posters on site | AS5.1

Data-driven global ocean model resolving atmospherically forced ocean dynamics 

Jeong-Hwan Kim, Daehyun Kang, Young-Min Yang, Jae-Heung Park, and Yoo-Geun Ham

Artificial intelligence has advanced global weather forecasting, outperforming traditional numerical models in both accuracy and computational efficiency. Nevertheless, extending predictions beyond subseasonal timescales requires the development of deep learning (DL)–based ocean–atmosphere coupled models that can realistically simulate complex oceanic responses to atmospheric forcing. This study presents KIST-Ocean, a DL-based global three-dimensional ocean general circulation model. Comprehensive evaluations confirmed the model’s robust ocean predictive skill and efficiency. Moreover, it accurately reproduces realistic ocean responses, such as Kelvin and Rossby wave propagation, and vertical motions induced by rotational wind stress, demonstrating its ability to represent key ocean–atmosphere interactions underlying climate phenomena, including the El Niño–Southern Oscillation. These findings reinforce confidence in DL-based global weather and climate models by demonstrating their capacity to capture essential ocean-atmosphere relationships. Building upon this foundation, the present study paves the way for extending DL-based modeling frameworks toward integrated Earth system simulations, thereby offering substantial potential for advancing long-range climate prediction capabilities.

How to cite: Kim, J.-H., Kang, D., Yang, Y.-M., Park, J.-H., and Ham, Y.-G.: Data-driven global ocean model resolving atmospherically forced ocean dynamics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16579, https://doi.org/10.5194/egusphere-egu26-16579, 2026.

EGU26-16636 | Posters on site | AS5.1

How can climate model emulators be aligned more closely with the needs of applied researchers? 

Nina Effenberger and Luca Schmidt

Earth System Models (ESMs) represent our most comprehensive tools for understanding and projecting climate change impacts; yet, they are highly computationally demanding and technically complex. Climate model emulators offer an alternative approach by approximating components or full ESM outputs at a reduced computational cost. Such emulators can range from reduced-order climate models to fully data-driven machine learning surrogates. As the demand for climate information increases, interest in climate model emulation has grown across both climate science and machine learning research, leading to rapid methodological development. Despite this shared interest, the two research fields remain largely disconnected and the application of machine learning climate emulators in climate science remains challenging [1]. Many emulators, therefore, remain unused in decision-making contexts--not because they lack value, but because methodological developers and users lack a shared framework for communication, evaluation, and practical guidance. 
This work examines this disconnect and takes a step towards facilitating the use of machine learning–based climate emulators in applied research and decision-making. We analyze and contrast methodological and applied perspectives on emulators, identify points of misalignment, and highlight opportunities for improved interaction. Building on these insights, we propose a tutorial-style framework that connects the two perspectives and provides practical guidance for developing, evaluating, and using climate emulators in research and decision-making contexts.

[1] Fowler, H. J., Mearns, L. O. and Wilby, R. L. [2025], Downscaling future climate projections: Compound-
ing uncertainty but adding value?, in ‘Uncertainty in Climate Change Research: An Integrated Approach’,
Springer, pp. 185–197.

How to cite: Effenberger, N. and Schmidt, L.: How can climate model emulators be aligned more closely with the needs of applied researchers?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16636, https://doi.org/10.5194/egusphere-egu26-16636, 2026.

EGU26-17080 | Posters on site | AS5.1

Deep learning-Based Global Ocean prediction model on the HEALPix Mesh 

Seonyu Kang, Yoo-Geun Ham, and Dongjin Cho

While deep learning-based atmospheric have been actively developed, in contrast, the development of ocean prediction models which allows multi-decade simulations through the autoregressive operation has been largely limited. This study developed a deep learning-based global ocean prediction model using the HEALPix grid system that capable of multi-decades integration in daily time step by successfully reproducing the observed global ocean statistics. Model training uses Fourier amplitude and phase losses to preserve low-frequency spatial structure and phase consistency, batch anomaly loss to learn anomalous variability, and sequentially ingests past-to-present atmospheric forcing to enable physically consistent coupled atmosphere–ocean dynamics in long-term integration. Long-term ocean model integration experiments with the observed atmospheric forcing demonstrate drift-free stable climatology for 20-yr simulations, with realistic Niño3.4 variations and ENSO-related global oceanic anomaly patterns consistent with observations. Furthermore, oceanic subsurface temperature responses to the westerly wind bursts (WWBs) over the equatorial western Pacific successfully capture the eastward propagation properties associated with the oceanic Kelvin waves.

How to cite: Kang, S., Ham, Y.-G., and Cho, D.: Deep learning-Based Global Ocean prediction model on the HEALPix Mesh, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17080, https://doi.org/10.5194/egusphere-egu26-17080, 2026.

EGU26-17113 | ECS | Posters on site | AS5.1

Evaluating machine learning approaches to improve observational daily precipitation datasets 

Skye Williams-Kelly, Lisa Alexander, Steefan Contractor, and Sahani Pathiraja

Accurate precipitation predictions are vital for water resource management and risk mitigation. Interpolated precipitation estimates derived from in situ observations are frequently used to evaluate climate models and analyse trends. However, these inadequately represent its spatio-temporal characteristics and significantly smooth out extremes, inhibiting effective evaluation of dynamical models and analysis of trends. Machine learning methods may be suited to addressing these limitations due to their ability to identify patterns in large datasets and use of GPU acceleration. Therefore, we compare three ML-based approaches for improving observational daily precipitation datasets: Gaussian Processes, Bayesian Neural Fields, and Neural Processes. Their performance is evaluated using traditional and distributional metrics, including on out-of-sample prediction, enabling an objective assessment of generalisation skill and representation of extremes. Results are further compared against existing precipitation products to identify the relative strengths and limitations of each method.

How to cite: Williams-Kelly, S., Alexander, L., Contractor, S., and Pathiraja, S.: Evaluating machine learning approaches to improve observational daily precipitation datasets, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17113, https://doi.org/10.5194/egusphere-egu26-17113, 2026.

EGU26-17600 | Orals | AS5.1

Rare event simulations, emulators, machine learning, and Bayesian GEV estimation, for predicting extreme heat waves and extremes of renewable electricity production 

Freddy Bouchet, Dorian Abbot, Laurent Dubus, Pedram Hassanzadeh, Amaury Lancelin, Jonathan Weare, Peter Werner, and Alexander Wikner

In the climate system, extreme events and tipping points (transitions between climate attractors) are of primary importance for understanding the impacts of climate change and for designing effective adaptation and mitigation strategies. Recent extreme heat waves with severe societal consequences, as well as prolonged periods of very low renewable energy production in electricity systems, are striking examples. A key challenge in studying such phenomena is the lack of available data: these events are inherently rare, and realistic climate models are computationally expensive and highly complex. This data scarcity severely limits the applicability of traditional approaches, whether based on modelling, physics, or statistical analysis.

In this talk, I will present new algorithms and theoretical approaches based on rare-event simulations, climate-model emulators, machine-learning methods for stochastic processes, and up to date blend of data and model use to estimate generalized extreme value (GEV) distribution. These methods are specifically designed to predict the probability that an extremely rare event will occur, to produce huge catalogues of dynamical trajectories leading to the event, and to use the best available historical and model data. The rare event simulation/emulator approach combines, on the one hand, state-of-the-art AI-based emulators that reproduce the full atmospheric dynamics of climate models, and, on the other hand, rare-event simulation techniques that reduce by several orders of magnitude the computational cost of sampling extremely rare events. In parallel the Bayesian GEV approach mix information from historical observation and CMIP model output to produce the best possible estimate of extreme event probabilities.

To illustrate the performance of these tools, I will present results on midlatitude extreme heat waves and on extremes of renewable energy production, with a particular focus on their implications for the resilience of electricity systems.

How to cite: Bouchet, F., Abbot, D., Dubus, L., Hassanzadeh, P., Lancelin, A., Weare, J., Werner, P., and Wikner, A.: Rare event simulations, emulators, machine learning, and Bayesian GEV estimation, for predicting extreme heat waves and extremes of renewable electricity production, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17600, https://doi.org/10.5194/egusphere-egu26-17600, 2026.

EGU26-18038 | ECS | Posters on site | AS5.1

Architectural Sensitivity of AI Weather Prediction Models to 3D Structural and Seasonal Climate Forcing 

Mozhgan Amiramjadi, Christopher Roth, and Peer Nowack

Data-driven weather prediction models have demonstrated remarkable skill, yet their ability to maintain a physically consistent three-dimensional atmospheric structure under out-of-distribution (OOD) conditions remains poorly understood. If OOD performance criteria could be met approximately, AI models would open up entirely new possibilities to generate large AI weather ensembles under future climate scenarios—for example, if initialized from climate model simulations (Rackow et al., 2024). This study conducts a multi-scale diagnostic evaluation of four state-of-the-art models—NeuralGCM (a deterministic hybrid model), GraphCast (a deterministic graph neural-network model), AIFS (a deterministic transformer-based model), and GenCast (an ensemble generative and diffusion-based model)—initialized across three distinct climate states: 1955 (cold), 2023 (neutral), sourced from ERA5 reanalysis, and 2049 (warm) simulated by the nextGEMS climate model (Segura et al., 2025).

Over 1–10-day leads, we find no detectable resolution-dependence for NeuralGCM's global skill, though the 1.4° configuration minimizes mean drift. A dominant spatial signature emerges across all models: a robust land–ocean contrast where oceans maintain smaller biases and slower Anomaly Correlation Coefficient (ACC) decay. Cross-hemispheric skill comparisons reveal that this contrast drives a significant asymmetry in error characteristics. In the 2049 warming scenario, the land-heavy Northern Hemisphere (NH, 39% land coverage) is the primary site of GraphCast's systematic "cool-drift" toward its training distribution, which peaks during boreal summer (JJA). In contrast, the generative GenCast model develops a pronounced warm bias localized in the oceanic Southern Hemisphere (SH, with about 20% land coverage).

For all three climate states, we further evaluate model performance across the entire troposphere and, as far as available, the stratosphere. While all four models maintain high variance-explained in the present-day mid-troposphere, performance degrades non-linearly under OOD forcing elsewhere, particularly within the stratosphere (< 200 hPa) and the boundary layer (> 900 hPa). Latitudinal R2-score cross-sections reveal that this degradation is most severe at polar latitudes; notably, in the 2049 scenario, GenCast exhibits a near-total collapse of skill by day 10, whereas NeuralGCM and GraphCast maintain localized predictive skill within the tropical troposphere.

The architecture-dependence of these simulated ensembles is confirmed by projecting day-10 drifts onto inter-climate "fingerprints" (T2049 - T2023 and T1955 - T2023). While AIFS and NeuralGCM show superior stability, GraphCast exhibits a systematic "cool-drift" toward its training climatology, and GenCast develops a distinct warm ocean drift. Beyond evaluating skill in surface variables, our results underline the need to assess data-driven models comprehensively across vertical, hemispheric, and seasonal diagnostics when applied to climate science scenarios, with implications for future AI model development.

References:

Rackow, T., et al (2024). Robustness of AI-based weather forecasts in a changing climate. arXiv preprint  arXiv:2409.18529. https://doi.org/10.48550/arXiv.2409.18529

Segura, H., et al. (2025). nextGEMS: entering the era of kilometer-scale Earth system modeling. Earth system modeling, Geosci. Model Dev., 18, 7735–7761, https://doi.org/10.5194/gmd-18-7735-2025

How to cite: Amiramjadi, M., Roth, C., and Nowack, P.: Architectural Sensitivity of AI Weather Prediction Models to 3D Structural and Seasonal Climate Forcing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18038, https://doi.org/10.5194/egusphere-egu26-18038, 2026.

EGU26-18557 | ECS | Posters on site | AS5.1

Bias-Correcting Arctic ERA5 Surface Air Temperatures using Deep Learning  

Sabine Scholle and Felix Pithan

Bias-Correcting Arctic ERA5 Surface Air Temperatures using Deep Learning 

Fine-tuning AtmoRep, a climate dynamics foundational model for improved Arctic 2m temperature predictions 

Due to the Arctic's harsh environment, comprehensive observational networks remain incomplete, leading to a reliance on biased reanalysis datasets such as ERA5. [1] This study investigates the potential of fine-tuning AtmoRep, a pre-trained transformer model for global atmospheric dynamics, to improve bias correction of Arctic 2-meter temperature (t2m) predictions. [2] 

Our methodology involves fine-tuning AtmoRep using ERA5 fields as input and bias-corrected Arctic t2m synthetic data, from a parallel project, as a target. [3] The project goal is to leverage AtmoReps global climate representations to further push the bias-corrected synthetic Arctic t2m data, given ERA5 as input (evaluated against observational data).

Preliminary results demonstrate stable validation performance of AtmoRep over the Arctic, achieving a t2m RMSE of 0.27 K during fine-tuning. Model robustness was further evaluated under severely masked target fields (up to 90% masking), and comparing BERT-style reconstruction with a forecasting-based training strategy. 

This study represents a novel application of foundation pretrained climate models for bias correction in sparsely observed Arctic regions, highlighting the potential of machine learning approaches to advance atmospheric science. 

  • Tian, T., Yang, S., Høyer, J. L., Nielsen-Englyst, P., & Singha, S. (2024). Cooler Arctic surface temperatures simulated by climate models are closer to satellite-based data than the ERA5 reanalysis. Communications Earth & Environment, 5(1). https://doi.org/10.1038/s43247-024-01276-z 
  • Lessig, C., Luise, I., Gong, B., Langguth, M., Stadtler, S., & Schultz, M. (2023b, August 25). AtmoRep: A stochastic model of atmosphere dynamics using large scale representation learning. arXiv.org. https://arxiv.org/abs/2308.13280 
  • Hossain, A., Keil, P., Grover, H., et al. Machine Learning Eliminates Reanalysis Warm Bias and Reveals Weaker Winter Surface Cooling over Arctic Sea Ice. ESS Open Archive . December 24, 2025.  https://doi.org/10.22541/essoar.176659533.30384251/v1 

How to cite: Scholle, S. and Pithan, F.: Bias-Correcting Arctic ERA5 Surface Air Temperatures using Deep Learning , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18557, https://doi.org/10.5194/egusphere-egu26-18557, 2026.

EGU26-19650 | ECS | Posters on site | AS5.1

Global Evaluation of Probabilistic AI Weather Forecasts Across Extremes and Regimes 

Marc Girona-Mata, Andrew Orr, and Richard Turner

Recent probabilistic machine learning weather forecasting models have demonstrated competitive skill relative to state-of-the-art (SOTA) numerical weather prediction ensemble systems. However, a rigorous global assessment of their skill, particularly in the distribution tails relevant for extremes as well as across different geographical regions, remains limited. Here, we present a systematic evaluation of various SOTA probabilistic AI weather forecasting systems against ECMWF’s Integrated Forecasting System Ensemble (IFS ENS), focusing on forecast skill across the full range of event intensities.

We analyse global forecasts at 24- and 72-hour lead times for near-surface temperature, 10 m wind speed, and total precipitation at 0.25° resolution over the 2024-2025 period. Forecasts are evaluated using the fair Continuous Ranked Probability Score (fCRPS) to account for differing ensemble sizes, as well as other complementary metrics. We also employ the threshold-weighted CRPS (twCRPS) computed for different quantiles ranging from the median up to the one-in-a-million extreme event. Scores are area-weighted and analysed both i) globally, ii) over land only, and iii) for different regions.

AI-based forecasts demonstrate comparable or improved probabilistic skill relative to the IFS ensemble in the bulk of the distribution, with particularly strong performance over tropical and mid-latitude oceans. However, skill systematically degrades at high quantiles for most variables, with more pronounced losses over land and at short lead times. Both diffusion- and CRPS-based probabilistic forecasts are competitive, but their relative skill varies across variables. Spatial diagnostics reveal coherent regime-dependent behaviour, with AI models underperforming in complex terrain and coastal regions where the IFS ENS retains a clear advantage. 

These results highlight both the promise and current limitations of probabilistic AI weather forecasting models, emphasising that headline global skill can mask substantial degradation in extreme-event and regional reliability.

How to cite: Girona-Mata, M., Orr, A., and Turner, R.: Global Evaluation of Probabilistic AI Weather Forecasts Across Extremes and Regimes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19650, https://doi.org/10.5194/egusphere-egu26-19650, 2026.

EGU26-19652 | ECS | Orals | AS5.1

Using process-based model simulations to develop and validate a data-driven approach for identifying climate drivers of maize yield failure 

Lily-belle Sweet, Christoph Müller, Jonas Jägermeyr, Weston Anderson, and Jakob Zscheischler

Climate impacts such as crop yield failure arise from complex combinations of weather conditions acting across multiple time scales, making it challenging to identify the most relevant climate drivers from high-resolution weather data. However, with data limitations, and the existence of complex and interacting relationships between growing-season climate conditions and plant growth, complex machine learning models that show high performance in predicting crop yield are often ‘right for the wrong reasons’. Process-based crop model simulations, which embody known functional relationships, could provide a useful testbed for developing and evaluating more trustworthy and robust methods. We present a novel two-stage, data-driven framework designed to extract a parsimonious set of climate drivers from multivariate daily meteorological inputs by systematically generating, evaluating and discarding candidate features using machine learning and then producing a set of drivers that are robust across locations, years and predictive feature combinations. We first validate the method using simulated U.S. maize yield failure data from two global gridded crop models, using rigorous out-of-sample testing: training on only early 20th-century data and holding out over 70 subsequent years for evaluation. The drivers identified using our approach align with known crop model mechanisms and rely solely on model input variables. Parsimonious logistic regression models built from these drivers achieve strong predictive skill under non-stationary climate conditions.

After validating the methodology on simulated data, we apply the same approach to observed county-level yields and daily multivariate weather data in rainfed and irrigated US maize systems. We identify compact sets of five climate drivers that effectively reproduce interannual variability and major historic failure events, including the 1993 Midwest floods and the 2012 drought. In rainfed systems, yield failure risk is strongly associated with extended periods of high soil moisture conditions after establishment, seasonal precipitation levels and vapor pressure deficit (VPD), with more than 40 high-VPD days between flowering and maturity markedly increasing odds of yield failure. In irrigated systems, critical drivers include soil moisture conditions surrounding planting, hot or dry days after establishment, and dewpoint temperatures near harvest. Our results demonstrate the transferability of the method from simulations to observations, and suggest its applicability to other crops, locations and further climate-related impacts. By avoiding reliance on post-hoc interpretability of black-box models, this framework enables the use of inherently interpretable, statistical models while still leveraging the predictive power of high-dimensional meteorological datasets.

How to cite: Sweet, L., Müller, C., Jägermeyr, J., Anderson, W., and Zscheischler, J.: Using process-based model simulations to develop and validate a data-driven approach for identifying climate drivers of maize yield failure, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19652, https://doi.org/10.5194/egusphere-egu26-19652, 2026.

EGU26-20173 | ECS | Posters on site | AS5.1

Exploring Adversarial Attacks in AI Weather Models for Generation of High-resolution Tropical Cyclones 

Marco Froelich and Sebastian Engelke

There has been recent interest in the advantage of differentiability of AI-weather models to enable direct computation of model sensitivities to initial conditions. In the field of machine learning, adversarial attacks leverage these sensitivities to influence the output of the prediction system by finding optimal initial condition perturbations. In weather forecasting, this methodology can be seen under two lenses: differentiable models are susceptible to malicious attacks aimed at distorting operational forecasts [1], while having access to sensitivities is an opportunity to further our understanding of real events through the generation of synthetic forecasts. Adversarial examples - perturbed initial conditions obtained from adversarial attacks - have been used in [2] to create even more extreme forecasts of a heatwave, providing a storyline approach to understanding black swan heatwave events. 

We further this effort by exploring adversarial attacks of tropical cyclone predictions at 0.25° resolution using Operational GraphCast. Although AI-weather models are known to improve tropical cyclone track predictions against numerical systems it remains challenging to forecast high intensities, particularly at high-resolution. Indeed, AI-weather models trained with MSE-type losses on reanalysis are known to suffer from 'blurred' forecasts due to the implicit down-weighing of small scale features. We find that while standard adversarial attacks of tropical cyclone forecasts are effective in controlling tropical cyclone tracks, they fail to reproduce realistic gradients of temperature, geopotential and wind fields, effectively worsening blurring effects. This is true also for attacks on the AMSE-finetuned Operational GraphCast model [3] which otherwise shows significant improvements in representing small scale features. We then borrow insights from the machine learning literature on the impact of the low-frequency bias of neural networks and its relationship to adversarial examples to improve this limitation and explore the capabilities of AI-weather models in global high-resolution tropical cyclone forecasting. 

 

References: 
[1] Imgrund, E., Eisenhofer, T., Rieck, K., 2025. Adversarial Observations in Weather Forecasting.
[2] Whittaker, T., Luca, A.D., 2025. Constructing Extreme Heatwave Storylines with Differentiable Climate Models.
[3] Subich, C., Husain, S.Z., Separovic, L., Yang, J., 2025. Fixing the Double Penalty in Data-Driven Weather Forecasting Through a Modified Spherical Harmonic Loss Function.

How to cite: Froelich, M. and Engelke, S.: Exploring Adversarial Attacks in AI Weather Models for Generation of High-resolution Tropical Cyclones, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20173, https://doi.org/10.5194/egusphere-egu26-20173, 2026.

EGU26-20724 | Orals | AS5.1

Machine learning identification of dry Intrusion outflows in present and future climates 

Jennifer Catto, Owain Harris, Stefan Siegert, and Shira Raveh-Rubin

Dry intrusions (DIs) are the key descending airstreams within extratropical cyclones. They can exacerbate the impacts of mid-latitude weather systems through their interactions with the boundary layer, enhancing atmosphere-surface interactions, and affecting frontal precipitation. DIs have been identified in the past using Lagrangian trajectory analysis, which has enabled studies into the climatology, variability, and characteristics of these airstreams. However, the potential futures of DIs, and the impact of climate change on them, has been unexplored due to the computational and data demands of this approach.

In this work, a convolutional neural network – DI-Net – is trained to identify DI outfow objects from a Lagrangian-identified dataset across the Northern Hemisphere, using information on relative and specific humidity, and topography from ERA5. The model performs well at capturing the main features of the DI climatology. DI-Net is then applied to historical and future climate model data from MRI-ESM2.0 to evaluate the climate model and investigate future changes. We present some of the challenges associated with developing a machine learning model for use with climate data.

The climate model represents the frequency of DIs well. In the most extreme warming scenario (SSP5-8.5), the frequency of DI outflows decreases in general, with increases across western Europe, consistent with the projections of the extratropical stormtracks seen in CMIP6 models. This study demonstrates the utility of the machine learning model to allow us to investigate the future of DIs, and eventually to understand more about how their impacts may change.

How to cite: Catto, J., Harris, O., Siegert, S., and Raveh-Rubin, S.: Machine learning identification of dry Intrusion outflows in present and future climates, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20724, https://doi.org/10.5194/egusphere-egu26-20724, 2026.

EGU26-21303 | Posters on site | AS5.1

Multiscale Graph Neural Networks for Climate Data Analysis 

Étienne Plésiat, Maximilian Witte, Johannes Meuer, and Christopher Kadow

We present a flexible deep learning framework for climate data analysis that leverages message-passing graph neural networks.

The framework is fully configurable and allows users to construct diverse architectures. In particular, it supports encoder-processor-decoder configurations in which geophysical fields are mapped onto a hierarchy of multi-icosahedral meshes, enabling information to propagate across scales before being mapped back to the original spatial grid. The model architecture is defined through a set of graph operators, including transformer-based graph convolutions. The framework operates on both regular and irregular grids, and enables flexible multivariate processing with spatial consistency. It further incorporates adaptive graph connectivity, enabling robust handling of missing data through dynamic edge construction. Additionally, several explainable AI (XAI) techniques are integrated to facilitate interpretation and physical attribution.

These features make the framework suitable for a broad range of climate and Earth-system applications, including data infilling, downscaling and process attribution. Its capabilities are illustrated through two case studies: (i) the reconstruction of global precipitation fields from incomplete observations, with comparison to established statistical and deep learning methods, and (ii) the attribution of large-scale drivers contributing to an extreme heatwave event.

The framework is currently being deployed as a web processing service that supports operational inference for selected climate applications.

How to cite: Plésiat, É., Witte, M., Meuer, J., and Kadow, C.: Multiscale Graph Neural Networks for Climate Data Analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21303, https://doi.org/10.5194/egusphere-egu26-21303, 2026.

EGU26-21336 | ECS | Posters on site | AS5.1

Performance of Spatiotemporal Causal Effect Estimation in Coupled Climate Models 

Rebecca Herman and Jakob Runge

Climate scientists are increasingly exploring the possible applications of artificial intelligence to climate modeling, whether for use inside the model to replace parameterized model components, or for use separately as an emulator of observed or simulated climate. However, a major limitation of standard artificial intelligence techniques is that they cannot distinguish between statistical association and causality. While this is not a drawback for the purpose of statistical prediction in an unchanging system, it can pose a problem for generalization of parameterizations and emulators under climate change, and furthermore, it means that it is not sound to use such techniques to predict the response of the climate system to unobserved interventions, including proposed climate engineering initiatives. The framework of causal inference attempts to address this limitation, providing techniques for discovering qualitative (“discovery”) and quantitative (“effect estimation”) information about the system’s response to interventions from purely observational data (or imperfect experiments) using causal reasoning. However, it was not originally developed for application to spatiotemporal dynamical systems such as the climate system.

In previous work, we develop a unified framework for causal effect estimation in spatiotemporal dynamical systems. In contrast to the hard interventions on univariate representations of coupled climate phenomena that until now have been more commonly used, our framework allows the user to investigate the effect of a spatiotemporal perturbation on a climate variable in one finite region on another variable in a different finite region at another time after specifying the qualitative causal relationships between the regions as a whole. This framework advances causal effect estimation for climate science because spatiotemporal perturbations are better defined, more actionable, and more interpretable than hard interventions on conceptual climate phenomena.

Here, we evaluate its performance using CMIP6-class models, focusing initially on the effect of the El Niño Southern Oscillation (ENSO) on the North Atlantic Oscillation as an example query. We assess the robustness of the method to data sample size, resolution, and other methodology choices by comparing the causal effect for a given model calculated from different subsets of its pre-Industrial control simulation using various amounts of spatial data and various values of other parameters of the algorithm. We use these results to assess the expected uncertainty on any inferences made using this technique from the short observational record or CMIP6 historical simulations, and make recommendations for best practices in different circumstances. Finally, we evaluate the accuracy of the predictions by using a causal model trained on historical simulations to predict the output of Tropical Basin Interaction Model Intercomparison Project experiments from the same climate model that nudge Pacific Sea Surface Temperature in the ENSO region in a manner comparable to our perturbation intervention.

How to cite: Herman, R. and Runge, J.: Performance of Spatiotemporal Causal Effect Estimation in Coupled Climate Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21336, https://doi.org/10.5194/egusphere-egu26-21336, 2026.

EGU26-226 | ECS | Orals | CL4.10

Assessment of climate change contribution to seasonal forecast anomalies  

Louis Ledoux--Xatard, Damien Specq, Saïd Qasmi, and Hervé Giordiani

Numerical seasonal forecasting consists in predicting the expected distribution of several climate variables (e.g. temperature, precipitation) over the next three months, using a global climate model that is initialized with real-time observations. Seasonal forecasts are often communicated as anomalies with reference to the model climatology estimated from forecasts initialized over a past period (hindcasts).

These anomalies are affected by long term trends due to anthropogenic climate change. Consequently, most seasonal forecasts of temperature currently issued by the Copernicus Climate change services (C3S) in the last few years indicate warmer than normal conditions over Europe, regardless of the season. 

Here, we investigate three methods to quantify the contribution of climate change from seasonal forecasts of temperature anomalies, and compare it to the usual reference based on hindcast climatology. First, we use a linear trend fitted on hindcasts. This approach is usually used in the literature to evaluate the forecast skill as it provides an estimate of the  climate change response. However, this method relies on the major assumption that the anthropogenic climate (forced) response is linear, which is not always reasonable. The second method is based on a Bayesian technique which combines CMIP6 simulations and seasonal hindcasts to estimate the forced response within the model, assuming that it is indistinguishable from the CMIP6 ensemble. The third method is based on numerical seasonal forecast experiments initialized in a so-called counterfactual world unaffected by anthropogenic forcings: dynamical initial conditions are the same as for the real, factual, seasonal forecasts, but the thermodynamic initial conditions correspond to a colder climate representative of the hindcast climatology. From this protocol, the climate change contribution can be estimated from the difference between the factual and the counterfactual forecasts. In this work, the three methods are implemented on the operational Météo-France seasonal forecast. While both the Bayesian method and numerical experiments show consistent results in the forced response estimate, results from the linear method might be inappropriate or overly simplistic in some cases.

How to cite: Ledoux--Xatard, L., Specq, D., Qasmi, S., and Giordiani, H.: Assessment of climate change contribution to seasonal forecast anomalies , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-226, https://doi.org/10.5194/egusphere-egu26-226, 2026.

EGU26-1319 | ECS | Orals | CL4.10

Trend Analysis and Forecasting of Climate in the Ladakh region of Western Himalayas using the Mann-Kendall test and Machine Learning models 

Saqib Iqbal Raina, Rayees Ahmed, Masood Ahsan Siddiqui, and Shahid Saleem

The cold-arid, high-altitude region of Ladakh is among the most climate-sensitive environments in the Western Himalayas, yet long-term assessments of its climatic trajectory remain limited. This study provides a comprehensive analysis of rainfall and temperature variability using IMD gridded data (1980–2024), combining the Mann–Kendall test, Sen’s slope estimator, and ensemble machine learning models (Random Forest and XGBoost) to detect past trends and forecast climate conditions for 2025–2054. Results reveal a significant and persistent decline in precipitation across all months and seasons, with an annual decrease of –47.13 mm/year. Winter and summer exhibit the sharpest reductions, highlighting weakening western disturbances that dominate Ladakh’s hydrometeorology. Maximum and minimum temperatures show robust warming, with Tmin rising more rapidly (+0.0175 °C/year) than Tmax (+0.0184 °C/year), indicating pronounced night-time warming and implications for permafrost and glacier stability. Machine-learning-based forecasts project continued aridification, with rainfall declining by 6–12% and winter Tmin increasing by +0.9 to +1.2 °C by 2054. XGBoost outperformed RF across all performance metrics, producing more stable and reliable predictions. The combined evidence points to warmer winters, reduced snow accumulation, altered meltwater timing, and heightened water stress in Ladakh’s fragile mountain environment. These findings underscore the urgent need for adaptive water-resource strategies, integration of advanced forecasting tools into regional climate services, and enhanced monitoring of cryosphere–climate interactions in the Western Himalayas.

Keywords: Ladakh; Climate variability; Mann–Kendall test; Sen’s slope; Rainfall trends; Temperature trends; Machine learning forecasting; Random Forest; XGBoost; High-altitude Himalaya.

How to cite: Raina, S. I., Ahmed, R., Siddiqui, M. A., and Saleem, S.: Trend Analysis and Forecasting of Climate in the Ladakh region of Western Himalayas using the Mann-Kendall test and Machine Learning models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1319, https://doi.org/10.5194/egusphere-egu26-1319, 2026.

EGU26-2450 | Orals | CL4.10

Prediction systems can forecast the direction of global stilling. 

Paul-Arthur Monerie, Jon I Robson, Reinhard Schiemann, Benjamin W Hutchins, and David J Brayshaw

The near-surface (10-m) wind speed (hereafter referred to as NSWP) is a key meteorological variable that contributes to the hydrological cycle, the transport of dust and plants, and the energy sector (e.g. wind energy). The NSWP decreased over the Northern Hemisphere (0–70°N) between 1980 and 2010. This decrease in the mean NSWP over the Northern Hemisphere is known as 'global stilling'. Using decadal predictions (DCPP-A, or Decadal Climate Prediction Project, Phase A), we demonstrate the feasibility of predicting the direction of global stilling for forecast lead times ranging from one to ten years. For example, prediction skill (quantified as the anomaly coefficient correlation, ACC) is high for the 2–5 year forecast lead time (ACC = 0.81). We demonstrate that this high prediction skill is due to the impact of changes in atmospheric greenhouse gas concentrations and anthropogenic aerosol emissions. However, the prediction of wind speed variability relative to the long-term downward trend is poor.

How to cite: Monerie, P.-A., Robson, J. I., Schiemann, R., Hutchins, B. W., and Brayshaw, D. J.: Prediction systems can forecast the direction of global stilling., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2450, https://doi.org/10.5194/egusphere-egu26-2450, 2026.

From the perspective of the annual harmonic, the role of heat capacity in controlling the seasonal cycle of surface temperature is readily apparent: a larger heat capacity means a greater phase delay between solar insolation and surface temperature, as well as a reduced amplitude. But how other processes, including latent and sensible heat fluxes, influence surface energy budget and thereby the seasonal cycle of temperature is not well understood.  

Here we use a linearisation of the surface energy budget to isolate how a range of processes influence the seasonal cycle of surface temperature. The theory highlights how surface wind speed and relative humidity can induce phase delays in surface temperature, analogous to the effect of heat capacity. The framework also quantifies how these variables can modify asymmetry in the seasonal cycle of surface temperature (i.e., differing lengths of warming and cooling seasons) from that expected from insolation alone. In addition to the linearisation approach, we perform simulations with an idealised climate model (“Isca”) to quantify the role of these processes in setting the overall phase and amplitude of the seasonal cycle of surface temperature. Implications of the theory and idealised simulations for understanding variations in the seasonal cycle of temperature across latitude, across surface types (e.g., land vs ocean), and across climate states are discussed. 

How to cite: Duffield, J. and Byrne, M.: Processes controlling the seasonal cycle of surface temperature: theory and idealised simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2773, https://doi.org/10.5194/egusphere-egu26-2773, 2026.

EGU26-3095 | ECS | Orals | CL4.10

Large potential of performance-based model weighting to improve decadal climate forecast skill 

Vincent Verjans, Markus Donat, Carlos Delgado Torres, and Timothy DelSole

Decadal climate predictions are sensitive to model initialization and simulation of climate forced response and internal variability. While analogue-based initialization selects initial states matching observations from large climate model ensemble simulations, it neglects differences in model performance. Focusing on sea-surface temperature decadal predictions, we couple analogue-based initialization with performance-based model weighting. Specifically, we favor selection of analogues from models that are statistically more consistent with observations in climate forced response and spatiotemporal variability characteristics. Through this statistical procedure, we demonstrate the effectiveness of a deviance metric that simultaneously evaluates multiple aspects of model-observation consistency and is novel to model weighting practices. We first conduct performance-weighted predictions of pseudo-observations, targeting model realizations instead of observations. Applying this exercise to more than 300 pseudo-observations to ensure robustness, we demonstrate large decadal forecast potential skill improvement compared to unweighted predictions. Second, we apply the same prediction method in decadal hindcasts of 95-year real-world sea-surface temperature observations. We find significant skill gains from performance-based weighting, however at considerably lower levels than in the pseudo-observation configuration. We explain this apparent contradiction by limited intrinsic predictability, similarity between unweighted and weighted ensembles, and inherent skill sampling uncertainties; we diagnose evidence for these three limitations in our results. Our analysis therefore highlights previously unrecognized challenges in validating performance-based model weighting, with implications for model weighting practices for climate predictions and projections across time scales.

How to cite: Verjans, V., Donat, M., Delgado Torres, C., and DelSole, T.: Large potential of performance-based model weighting to improve decadal climate forecast skill, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3095, https://doi.org/10.5194/egusphere-egu26-3095, 2026.

EGU26-3266 | ECS | Orals | CL4.10

Multi-year La Niñas Break the Interannual Symmetric GMST Responses to Strong ENSO Events 

Ke-Xin Li, Fei Zheng, Jin-Yi Yu, Lin Wang, and Jiang Zhu

Strong El Niño and La Niña events typically produce symmetric impacts on global mean surface temperature (GMST), inducing notable warming or cooling, respectively, from their developing year through the boreal summer of the following year. However, this symmetry in GMST response breaks down in the subsequent autumn and winter, and the underlying mechanism has remained unclear. This study reveals that the opposite transition behaviors of strong ENSOs are key to this breakdown: while strong El Niños commonly transition into La Niña, strong La Niñas more often persist into multi-year episodes, resulting in asymmetric climate trajectories. These divergent evolutions produce asymmetric GMST anomalies since post-summer, including not only the divergent locations and intensities of cold sea surface temperature over tropical Pacific, but also the contrasting land surface temperature dipoles over the Northern Hemisphere’s mid-to-high latitudes, mediated by tropical–extratropical teleconnections. These findings highlight a previously underappreciated source of GMST variability and offer new insight into its predictability on interannual–biennial timescales.

How to cite: Li, K.-X., Zheng, F., Yu, J.-Y., Wang, L., and Zhu, J.: Multi-year La Niñas Break the Interannual Symmetric GMST Responses to Strong ENSO Events, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3266, https://doi.org/10.5194/egusphere-egu26-3266, 2026.

Atlantic multidecadal variability (AMV) has profound climate impacts on both local and remote areas. Traditional analyses mostly concentrated on the AMV impacts on decadal-multidecadal variability. Recent studies show that AMV could also exert significant impacts on El Nino-Southern Oscillation (ENSO) and its connection with the Indian ocean dipole. However,  little attention has been paid to the AMV impacts on seasonal predictability. Based on observations and sets of ensemble hindcast products, for the first time, this study investigates the role of AMV phase on the seasonal predictability of sea surface temperature anomalies (SSTA) in North Atlantic. Our results show that the seasonal prediction skill and potential predictability of spring SSTA over the subtropical North Atlantic (STNA) region is significantly higher in AMV+ than in AMV- period. Similar contrasts between AMV phases are also obtained by the persistence skill of the observed SSTA over STNA at various lead months. Further analyses show that the differed seasonal predictability between different AMV phases are closely connected to the different upper ocean heat content, which is primarily contributed by different heat convergence driven by the Atlantic meridional overturning circulation.

How to cite: Wei, B. and Yan, X.: Seasonal predictability of North Atlantic sea surface temperature under different AMV phases, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4613, https://doi.org/10.5194/egusphere-egu26-4613, 2026.

EGU26-5458 | Orals | CL4.10

The road to 500 years of multi-member, seasonal climate hindcasts 

Martin Wegmann and Stefan Brönnimann

Understanding potential drivers of seasonal prediction skill as well the non-stationarity behaviour of prediction skill itself over time is key to the development of a trustworthy, operational climate forecast system. That said, most prediction systems, either statistical or physical, are tuned on the climate of the last 30-40 years. Going into a new climate state, it is important to evaluate the underlying predictability assumptions over multiple climate states.

We present initial output of a data set version 1.0, which covers the years 1421-2008 C.E., has 100 members for each forecast step, covers the variables sea level pressure, 2m temperature and 500 hPa geopotential height and will be produced for the months January, February, June, July, August and December. This data set is produced using rather simple convolutional neural networks as architecture (same as in the initial WeatherBench approach) and is trained on reanalysis-infused atmosphere-ocean general circulation model data.

Exchanging parts of the model chain, such as model architecture, training data and initial conditions will allow the community to develop better and better versions of this data set eventually.

This data set and its future versions should be understood as an open-science, community-driven project. The code and output data behind this data set will be published openly. An exchange platform for interested community members will be highlighted during the presentation.

How to cite: Wegmann, M. and Brönnimann, S.: The road to 500 years of multi-member, seasonal climate hindcasts, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5458, https://doi.org/10.5194/egusphere-egu26-5458, 2026.

EGU26-5956 | ECS | Orals | CL4.10

Mechanisms driving Subpolar North Atlantic Upper Ocean Heat Content Predictability in CMIP6 Decadal Prediction Systems 

Dylan Oldenburg, Stephen Yeager, Gokhan Danabasoglu, Isla Simpson, and Who Kim

Previous work has indicated that the subpolar North Atlantic Ocean exhibits particularly high decadal predictability, influenced by both external forcing and predictable internal variability as a result of large-scale ocean processes. The mechanism driving subpolar North Atlantic (SPNA) upper ocean heat content (UOHC) predictive skill identified in the Decadal Prediction Large Ensemble of CESM (CESM-DPLE) is linked to predictable barotropic gyre and AMOC circulations, with the ocean memory linked to the Labrador Sea Water (LSW) thickness, further corroborated by other studies. Here, we investigate whether this mechanism holds in CMIP6 decadal prediction systems with variable SPNA UOHC skill by analysing lagged regressions between initial LSW deep density and AMOC, sea-surface height, the barotropic streamfunction, deep ocean density, and UOHC. We further investigate lagged regressions between the deep ocean density in the Irminger-Iceland Basins (IIB) and these same variables to determine whether some models show a stronger connection between the SPNA UOHC and the IIB density. We have determined that models with higher SPNA UOHC skill tend to exhibit stronger correlations between the SPNA UOHC at later years and the initial LSW density (i.e., the density at the first month after initialisation). However, high model predictive skill in this initial density is not necessarily associated with higher skill in the subsequent SPNA UOHC. In higher skill models, such as CESM2-DP, CESM1-DP and HadGEM3-GC31-MM, densification in the deep Labrador Sea (1000m-2500m) is associated with a near-simultaneous increase in the AMOC strength and spin up of the subpolar gyre (SPG) as well as a subsequent warming in the subpolar North Atlantic, which later spreads to the western SPG as well. In these models, deep density anomalies accumulate between 1000m-2500m and propagate eastwards at 45°N. In low-skill models, such as CanESM5, IPSL-CM6A-LR, FGOALS-f3-L or BCC-CSM2-MR, LSW densification exhibits either no link to AMOC strength or yields only a brief period of strong AMOC, and is not associated with a persistent warming pattern in the SPNA at later years in the simulations. In these models, density anomalies at depth at 45°N appear in the initial years, but dissipate rapidly and do not propagate eastwards.

How to cite: Oldenburg, D., Yeager, S., Danabasoglu, G., Simpson, I., and Kim, W.: Mechanisms driving Subpolar North Atlantic Upper Ocean Heat Content Predictability in CMIP6 Decadal Prediction Systems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5956, https://doi.org/10.5194/egusphere-egu26-5956, 2026.

In this study, we apply the Model‑based Analog Forecast (MAF) approach to perform Indian Ocean Dipole (IOD) hindcasts using CMIP6 pre‑industrial simulations. The MAF method constructs forecast ensembles by identifying states in existing model simulations that best match an observed initial anomaly and then tracing their subsequent evolution, without requiring additional model integrations. By optimizing key parameters in the MAF framework, we demonstrate that the MAF‑based IOD hindcasts exhibit skill comparable to that of assimilation‑initialized hindcasts. Utilizing this approach, we investigate the diversity in IOD prediction skill across different climate models, with a focus on the impact of cold tongue bias on forecast performance. Our analysis reveals substantial inter‑model spread in IOD prediction skill within CMIP6 models, with useful predictability extending up to 1–4 months depending on the model. Furthermore, we identify a clear link between cold tongue bias and IOD prediction skill: models with a stronger cold tongue bias show weaker El Niño–Southern Oscillation (ENSO) teleconnections into the tropical Indian Ocean, which consequently reduces their IOD forecast capability. These results offer valuable insights into the sources of IOD prediction diversity and underscore potential pathways for improving IOD forecasting.

How to cite: Wu, Y.: Assessing the Impact of Cold Tongue Bias on IOD Predictability Using a Model-Analog Method, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6147, https://doi.org/10.5194/egusphere-egu26-6147, 2026.

EGU26-7969 | Posters on site | CL4.10

Comparison of Correction Methods for Seasonal Forecasts of Temperature over Central Europe 

Maciej Jefimow, Kinga Kulesza, Joanna Strużewska, Karol Przeździecki, and Aleksandra Starzomska

The direct applicability of seasonal forecasts is limited by their coarse spatial resolution, an issue that is particularly visible in mountainous regions. Therefore, post-processing procedures are required to improve forecast quality and obtain results suitable for regional-scale applications.

In this study, we compare two correction methods for improving seasonal forecasts of 2-meter air temperature (T2m): quantile mapping and vertical temperature correction using a lapse-rate approach. We use seasonal forecast outputs from the ECMWF model provided by the Copernicus Climate Change Service (C3S), with the domain restricted to Central Europe and centred over Poland (13–26°E, 47.5–55°N).

ERA5 reanalysis data were used for a 10-year training period in the quantile mapping procedure, which is based on non-parametric, robust empirical quantiles and applied independently at each grid point. In parallel, a simple physically based correction incorporating vertical temperature lapse rates was evaluated.

Forecast performance was assessed for selected months. Preliminary results indicate that the lapse-rate-based correction outperforms quantile mapping in reproducing local temperature patterns over the study area.

How to cite: Jefimow, M., Kulesza, K., Strużewska, J., Przeździecki, K., and Starzomska, A.: Comparison of Correction Methods for Seasonal Forecasts of Temperature over Central Europe, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7969, https://doi.org/10.5194/egusphere-egu26-7969, 2026.

EGU26-9079 | Posters on site | CL4.10

Tailored seasonal climate forecasts for crop breeding in the Nordic and Baltic regions  

Andrea Vajda and Otto Hyvärinen

As climate change drives a northward shift in agro-climatic zones across Europe, it presents both risks and opportunities for agricultural production in the Nordic regions. Plant breeding plays a key role in adaptation strategies by enabling the development of climate-resilient crop varieties and exploiting novel growing conditions to secure yields. The NorBalFoodSec project aims at increasing food security in the Nordic and Baltic regions by advancing knowledge on how to better adapt crop breeding and agricultural production to future climates. As part of this effort, tailored seasonal climate forecasts for agri-food production are developed and their applicability and value in supporting crop breeders’ planning and decision-making in crop management are evaluated.  In this study, the predictability of key variables, i.e. temperature and precipitation for growing season, and the reliability assessment of the developed seasonal forecasts tailored for agri-food productions are presented.

To investigate the predictability limits of seasonal forecasts in the Nordic and Baltic region, we post-processed and evaluated the skill of temperature and precipitation from ECMWF’s SEAS5 seasonal forecast system using reforecasts for 1981-2016 and the ERA5 reanalysis dataset as reference. The analysis employed the open source CSTools package for R, which implements widely used methods from literature, ranging from the simple bias removal to the ensemble calibration methods that correct the bias, the overall forecast variance and ensemble spread. For precipitation, downscaling approaches such as the RainFarm stochastic method were tested to generate and assess higher-resolution fields. Furthermore, we explored EMOS (ensemble model output statistics), a nonhomogeneous regression technique widely used in short-range weather forecasting but less common in the post-processing of longer-range forecasts. Based on verification results, the most effective bias adjustment methods were applied to reduce the systematic errors in temperature and precipitation.

The post-processed variables were then used to develop growing season indicators, selected in close collaboration with crop breeders to meet their specific needs, such as the start of growing season, growing degree days, mean temperature, total precipitation and dry spell. The value of these seasonal forecasts is assessed using historical forecasts for 2017-2026 with a focus on years featuring hazardous conditions for key crops: cereal (barley), forage (red clover) and tubers (potatoes). Ultimately, these forecasts aim to support crop breeders in planning and decision-making for improved crop management.

How to cite: Vajda, A. and Hyvärinen, O.: Tailored seasonal climate forecasts for crop breeding in the Nordic and Baltic regions , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9079, https://doi.org/10.5194/egusphere-egu26-9079, 2026.

EGU26-9243 | Orals | CL4.10

Underestimated Extended Seasonal Hindcast Skill in Sparsely Observed Periods Revealed Through Hybrid Machine-Learning Initialization 

Goratz Beobide-Arsuaga, Jürgen Bader, Simon Lentz, Sebastian Brune, Christopher Kadow, and Johanna Baehr

The North Atlantic is a key source of seasonal-to-interannual climate predictability, as Subpolar Gyre (SPG) sea surface temperature anomalies (SSTAs), coupled with the North Atlantic Oscillation (NAO), modulate surface air temperatures over Europe and North America. However, model biases in North Atlantic dynamics and ocean–atmosphere coupling limit the skill of initialized hindcasts. While data assimilation partially constrains these errors using observations, hindcasts initialized during periods of sparse observational coverage may underestimate the true predictive potential of the system. Here, we reassess North Atlantic-driven extended seasonal predictability for the period 1960-2020 using a hybrid machine-learning (ML) assimilation approach, trained during periods with abundant observations (2004-2020) and applied to reconstruct North Atlantic Ocean temperatures during sparsely observed periods (1960-2004). Relative to standard initialization, the hybrid ML approach leads to stronger ocean–atmosphere coupling and a more robust NAO-like atmospheric response. As a result, we find enhanced winter and spring SSTA skill in the SPG during the first lead year in sparsely observed periods, along with improved surface air temperature skill over northwestern North America, southern Greenland, and central to northern Europe. Our results suggest that initialized prediction systems may systematically underestimate North Atlantic-driven predictability, and that initialization improved by hybrid ML can unlock greater forecast credibility than is implied by current standard hindcasts.

How to cite: Beobide-Arsuaga, G., Bader, J., Lentz, S., Brune, S., Kadow, C., and Baehr, J.: Underestimated Extended Seasonal Hindcast Skill in Sparsely Observed Periods Revealed Through Hybrid Machine-Learning Initialization, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9243, https://doi.org/10.5194/egusphere-egu26-9243, 2026.

EGU26-9265 | ECS | Orals | CL4.10

Decadal predictions of wind and solar power indicators to support the renewable energy sector 

Sara Moreno Montes, Carlos Delgado-Torres, Matías Olmo, Sushovan Ghosh, Verónica Torralba, and Albert Soret

Renewable energy production is strongly influenced by weather and climate states, making the energy sector highly sensitive to climate variability from seasonal to decadal timescales. Decadal climate predictions, which forecast climate variability over the next 1–10 years, are therefore promising tools for optimising renewable energy deployment. For example, reliable long-term forecasts can support the identification of the most suitable locations for wind farms and solar plants, helping to stabilize energy production and reduce climate-related risks.

This study assesses the predictive skill of decadal climate predictions for energy-relevant climate impact indicators, focusing on forecast years 1-3 over Western Europe. Climate indicators are used to quantify the impact of climate variability on energy production, which is ultimately the most useful information for the energy industry.  

The calculation of the indicators requires different climate variables and temporal resolutions depending on the energy source. For solar energy, daily mean values of near-surface air temperature (TAS), surface solar radiation (RSDS), and surface wind speed (SFCWIND) are used. For wind energy, 6-hourly SFCWIND is required. The indicators are computed using a multi-model ensemble from climate forecast systems participating in the Decadal Climate Prediction Project (DCPP), which is part of the Coupled Model Intercomparison Project Phase 6 (CMIP6). To evaluate the forecast quality of the indicators, the ERA5 reanalysis is used as the reference dataset during the period 1961-2019. Skill is evaluated against ERA5 and compared with non-initialized historical forcing simulations produced with the same models to quantify the added value of decadal initialization.

Three indicators are considered: photovoltaic potential (PVpot) for solar energy, capacity factor (CF) for wind energy, and the number of effective days (Neff) for both renewable energy resources. PVpot quantifies photovoltaic performance relative to nominal capacity and is derived from RSDS, TAS, and SFCWIND. Wind CF represents the ratio between actual and maximum possible energy production and depends on SFCWIND and turbine characteristics. Neff is defined as the number of days meeting efficiency-related thresholds for each resource, based on radiation and temperature constraints for solar PV technology and wind-speed limits associated with CF ≥ 25% and turbine cut-out for wind energy. By expressing production in terms of effective days, the Neff indicator enables anticipating periods when both renewable energy resources are simultaneously scarce, as well as a consistent cross-resources comparison between them.

Results show higher and more seasonally dependent skill for PVpot than for wind CF, with Neff skill varying across regions and seasons. Decadal initialization generally enhances skill in regions where historical simulations already exhibit predictability, while limited additional skill is introduced elsewhere, suggesting that initialization primarily amplifies existing sources of predictability rather than introducing entirely new skill. These results highlight the potential of tailored climate impact indicators to bridge decadal climate prediction science and renewable-energy applications.

How to cite: Moreno Montes, S., Delgado-Torres, C., Olmo, M., Ghosh, S., Torralba, V., and Soret, A.: Decadal predictions of wind and solar power indicators to support the renewable energy sector, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9265, https://doi.org/10.5194/egusphere-egu26-9265, 2026.

EGU26-9858 | ECS | Posters on site | CL4.10

Recalibrating counts of extreme temperature days in decadal predictions  

Samira Ellmer, Felix Fauer, Andy Richling, Luca Rolle, and Henning Rust

Decadal prediction models mostly focus on predicting mean temperatures and precipitation on annual scales. For applications in agriculture and the health sector, indicators for heat stress and extreme temperatures appear to be more relevant than the mean temperatures. Those indices often involve maximum temperatures on a daily scale. Decadal predictions need to be recalibrated to reduce biases and adjust dispersion to match prediction uncertainty and hence increase reliability. In the frame of the research project "Coming Decade", funded by the German Ministry of Research, Technology and Space, we explore two different approaches to obtain recalibrated probability distributions for the annual counts of days with maximum temperatures exceeding a given threshold, i.e. Summer Days (Tmax25°C) and Hot Days (Tmax≥30°C).

(1) First, we obtain annual counts of Summer Days and Hot Days directly from decadal predictions of daily maximum temperatures. Subsequently, we recalibrate the distribution of counts from the ensemble forecast using a variant of the parametric Decadal Climate Forecast Recalibration Strategy (DeFoReSt) proposed by Pasternack et al. (2018) with distributions accounting for count data, i.e. Poisson or negative-binomial distribution.

(2) As an alternative approach, we apply a bias and drift adjustment of daily maximum temperatures using non-homogeneous Gaussian regression in the frame of generalized additive models. From the resulting adjusted daily temperatures we obtain counts for daily exceedances and aggregate them to an annual scale. We then recalibrate with the ensemble recalibration strategy (1).

We aim to compare these approaches for recalibrated Summer Days and Hot Days over Europe using a skill score for probabilistic forecasts like the CRPSS. We use decadal predictions from the operational decadal prediction system of the German Meteorological Service (DWD) based on the Max Planck Institute Earth System Model (MPI-ESM1.2-LR) and evaluate the performance with respect to the ERA5 reanalysis.

How to cite: Ellmer, S., Fauer, F., Richling, A., Rolle, L., and Rust, H.: Recalibrating counts of extreme temperature days in decadal predictions , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9858, https://doi.org/10.5194/egusphere-egu26-9858, 2026.

EGU26-10491 | ECS | Orals | CL4.10

Unprecedented suppression of local upwelling in the Gulf of Panama predicted a season in advance 

Ronan McAdam, Antonella Sanna, and Enrico Scoccimarro

Wind-driven upwelling of subsurface ocean waters to the surface is a fundamental component of ocean dynamics, and ensures nutrient-rich waters reach the epipelagic zone. Weakening or collapse of upwelling can reduce nutrient availability, potentially impacting ecosystem health and fishing activities. In early 2025, the Gulf of Panama experienced an unprecedented collapse of the local upwelling system, indicated by exceptionally weak northerly winds leading to record warm ocean temperatures and reduced nutrient availability. Despite the societal relevance of this local-scale process, the predictability of upwelling strength and in particular collapse, remains poorly understood. 

Here, we explore the predictability of upwelling in the Gulf of Panama on seasonal timescales, and find that the unprecedented collapse of 2025 was accurately predicted a season in advance. We employ the operational seasonal forecasting system CMCC-SPS4 which has a horizontal resolution of 0.25o for the ocean component, 75 vertical depth levels, and outputs 40 ensemble members. Forecasts of sea surface temperatures initialised in November and December of 2024 predicted record values for January to March 2025, indicating considerable weakening of upwelling. Validation against the OSTIA sea surface temperature dataset using hindcasts from 1993 to 2024 demonstrates high probabilistic and deterministic skill, including for predictions of upper-quintile temperature events. Moreover, by validating against the global 1/12o GLORYS12 ocean reanalysis, we also find an increase in temperature forecast skill with depth, making the case for exploiting subsurface information for improved early-warning. 

While high surface temperatures are often used as an indicator of upwelling collapse, we show that in 1998—despite strong winds and active upwelling—extreme temperatures occurred throughout the water column. These results suggest that surface temperature records alone may not fully capture changes in nutrient availability. To ensure that the forecast system captures the collapse of upwelling, we also explore the predictions of regional winds and derived upwelling indicators. 

This study demonstrates the utility of seasonal forecasting in local marine environments and makes the case for future uptake in activities related to the Blue Economy. The work also supports the definition of user-relevant indicators of extreme temperatures (Horizon Europe project “ObsSea4Clim”) and the role of reanalyses in studying subsurface temperature extremes (as part of the ocean reanalysis validation project “GLORAN”).

How to cite: McAdam, R., Sanna, A., and Scoccimarro, E.: Unprecedented suppression of local upwelling in the Gulf of Panama predicted a season in advance, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10491, https://doi.org/10.5194/egusphere-egu26-10491, 2026.

EGU26-10937 | ECS | Posters on site | CL4.10

Effect of SST change of the Mediterranean sea and Atlantic Ocean over Western Europe over a 30-years period 

Clement Blervacq, Kazim Sayeed, Manuel Fossa, Nicolas Massei, and Luminita Danaila

With climate change accelerating, a key open question is how ocean warming will modulate regional atmospheric conditions. Sea-surface temperature (SST) is a major boundary condition forcing for the atmosphere, influencing near-surface temperature, humidity, and precipitation. We quantify the atmospheric response to prescribed SST warming using a suite of long, convection-permitting regional climate simulations with the Weather Research and Forecasting (WRF) model.

We performed 7 continuous simulations spanning 1996–2024 (29 years), centered on France and Western Europe, with a horizontal resolution of 20 km (90 × 80 grid points). One of the simulations serves as a baseline/reference case. The remaining six experiments impose SST perturbations designed to emulate end-of-century warming and to isolate the role of different basins. They form two families: (i) warming applied to the Mediterranean Sea only, and (ii) warming applied to both the Mediterranean Sea and the Atlantic Ocean. Within each family, three SST-forcing scenarios are considered: (1) mean SST anomalies representative for the year 2100 under RCP4.5, (2) mean SST anomalies representative for 2100 under RCP8.5, and (3) a “trend-shift” case in which SSTs are localy offset by the observed/prescribed multi-decadal SST increase, effectively shifting boundary conditions toward a warmer future.

We compare all experiments with the reference simulation to diagnose the regional climate's sensitivity to SST warming, focusing on near-surface air temperature and precipitation. The analysis distinguishes the magnitude of the response and the relative contributions of Mediterranean versus Atlantic warming, providing a controlled assessment of basin-specific SST impacts on Western European climate over multi-decadal timescales. The first conclusion is that, for RCP 4.5 and 8.5, the land temperatures show little change on average. However, when only the Mediterranean Sea is heated, a temperature anomaly of up to 5°C occurs north of the Atlantic Ocean. Further analysis is underway as the simulations run.

How to cite: Blervacq, C., Sayeed, K., Fossa, M., Massei, N., and Danaila, L.: Effect of SST change of the Mediterranean sea and Atlantic Ocean over Western Europe over a 30-years period, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10937, https://doi.org/10.5194/egusphere-egu26-10937, 2026.

EGU26-12228 | ECS | Orals | CL4.10

A Hybrid NWP–LSTM Framework for Seasonal Wind Speed Forecasting with Multi-Resolution Downscaling and Bias Correction 

Yaswanth Pulipati, Sachin S Gunthe, Balaji Chakravarthy, Swathi Vs, and Athul Cp

Reliable seasonal forecasting of near-surface wind speeds is essential for optimizing renewable energy production, particularly in regions with expanding wind power infrastructure. Global seasonal forecast models, despite offering valuable large-scale predictability, are limited by coarse resolution (~1°), which fails to resolve local topographic, land-surface, and boundary-layer influences critical for accurate hub-height wind predictions. This study presents a high-resolution dynamical downscaling framework using the Weather Research and Forecasting (WRF) model to enhance seasonal wind speed forecasts over a target region in India. Initial intercomparison of leading global seasonal systems (ECMWF SEAS5 and NCEP CFSv2) demonstrated superior performance by ECMWF SEAS5 in reproducing observed wind climatology over the Indian subcontinent, leading to its selection as the primary driving dataset. A three-domain WRF configuration (27 km → 9 km → 3 km) was implemented, and comprehensive sensitivity experiments identified the MYNN planetary boundary layer (PBL) scheme as the optimal configuration, yielding the lowest wind speed bias and best representation of vertical wind shear.

Downscaled hindcast simulations were rigorously validated against ERA5 reanalysis across multiple vertical levels, showing substantial improvements in hub-height wind speed skill metrics. To extend forecast skill beyond the 7-month limit of available boundary conditions, a long short-term memory (LSTM) neural network was developed and trained on 40 years of ERA5 wind time series using a sliding-window approach (7-month input → 90-day output). The model was retrained for each sliding window to adapt to evolving patterns, resulting in robust predictive performance from months 8 to 10. Finally, quantile mapping bias correction was applied to the downscaled and LSTM-extended outputs compared to ERA5, resulting in an approximately 38% reduction in root mean square error and a marked improvement in probabilistic reliability. The resulting bias-corrected, high-resolution seasonal wind speed dataset provides enhanced accuracy for wind resource assessment, power production forecasting.

How to cite: Pulipati, Y., Gunthe, S. S., Chakravarthy, B., Vs, S., and Cp, A.: A Hybrid NWP–LSTM Framework for Seasonal Wind Speed Forecasting with Multi-Resolution Downscaling and Bias Correction, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12228, https://doi.org/10.5194/egusphere-egu26-12228, 2026.

EGU26-15785 | Posters on site | CL4.10

Sources of biases in climate prediction: role of initial condition uncertainties of external forcing 

Stéphane Vannitsem and Wansuo Duan

Biases are often associated either to the presence of model structural errors or to a misrepresentation of the properties of initial condition errors (initial error biases or a bad representation of the initial error distribution). In the current work, the development of biases is addressed by considering a twin experiment in which the dominant initial condition uncertainties are imposed to the external forcing of a coupled ocean-atmosphere extratropical system in a perfectly controlled environment. The forcing is generated by a low-order 3-variable tropical model mimicking the dynamic of ENSO. No structural model errors are introduced and the statistical properties of the initial error are perfectly known. It is shown that even if this almost perfect setting, important biases are induced on seasonal-to-decadal forecasts, and hence unreliable (under-dispersive) ensembles.

More specifically, three main types of ensemble forecast experiments are performed: with random perturbations along the three Lyapunov vectors of the tropical model; along the two dominant Lyapunov vectors; and along the first Lyapunov vector only. When perturbations are introduced along all vectors, important forecasting biases, inducing a mismatch between the error of the ensemble mean and the error spread, are produced. Theses biases are considerably reduced only when the perturbations are introduced along the dominant Lyapunov vector. Hence, perturbing along the dominant instabilities allows a reduced mean square error to be obtained at long lead times of a few years, as well as reliable ensemble forecasts across the whole time range. These very counterintuitive findings, reported in Vannitsem and Duan (2026), further underline the importance of appropriately controlling the initial condition error properties in the tropical components of models.

Reference

Vannitsem, S., Duan, W. A Note on the Role of the Initial Error Structure in the Tropics on the Seasonal-to-Decadal Forecasting Skill in the Extratropics. Adv. Atmos. Sci. 43, 157–169 (2026). https://doi.org/10.1007/s00376-025-4521-7

How to cite: Vannitsem, S. and Duan, W.: Sources of biases in climate prediction: role of initial condition uncertainties of external forcing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15785, https://doi.org/10.5194/egusphere-egu26-15785, 2026.

EGU26-16000 | Posters on site | CL4.10

On the role of spiciness in Pacific Decadal Variability 

Vera Stockmayer, Niklas Schneider, Malte F. Stuecker, and Antonietta Capotondi

Decadal modulations of the tropical Pacific impact the weather and climate worldwide and modulate the rate of change of the global warming trend. However, the mechanisms driving these long-term changes, especially the role of subsurface ocean dynamics, remain debated. By connecting the extratropical and tropical Pacific, the upper-ocean circulation may act as a low-pass filter of stochastic wind forcing, providing a source of memory on decadal time scales. Here, we investigate the role of spiciness (i.e., density compensated temperature and salinity) anomalies as one possible driving mechanism of Tropical Pacific Decadal Variability (TPDV). Based on 100 realizations of the Community Earth System Model Version 2 - Large Ensemble (CESM2-LE), we construct a Linear Inverse Model (LIM), which highlights the coupling at decadal time scales between the subtropics and the equatorial Pacific by propagating spiciness anomalies and suggests a link to TPDV. The eigenmodes of the LIM (i.e., the Principal Oscillation Patterns) reveal distinct spiciness pathways with decadal time scales, accompanied by corresponding decadal SST signals in the tropics. Spiciness signals originating in the Southern Hemisphere indicate the strongest response of the equatorial Pacific with warm and salty equatorial spiciness anomalies corresponding to a positive equatorial SST anomaly. However, the exact contribution of the spiciness mechanism needs to be further quantified, as well as the contribution of other pycnocline processes linked to extratropical atmospheric forcing. 

How to cite: Stockmayer, V., Schneider, N., Stuecker, M. F., and Capotondi, A.: On the role of spiciness in Pacific Decadal Variability, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16000, https://doi.org/10.5194/egusphere-egu26-16000, 2026.

EGU26-16494 | Posters on site | CL4.10

The NAO decadal predictability determined by initial ocean heat content anomalies in the subpolar North Atlantic — SST gradients playing a key role. 

Panos J. Athanasiadis, Dario Nicolì, Domenico Giaquinto, Casey Patrizio, Stephen Yeager, Leon Hermanson, and Holger Pohlmann

In recent studies using large ensembles, the North Atlantic Oscillation (NAO) has been shown to exhibit significant decadal predictability stemming from skillfully predicted sea surface temperature (SST) anomalies in the subpolar North Atlantic (SPNA).  In turn, various studies have demonstrated that the decadal SST predictability in this area is dominantly due to ocean initialization. It remains unclear, however, which component of the oceanic initial conditions determines the evolution of the SPNA SSTs and the NAO in the following years, and through which physical processes this is accomplished.

Here we assess the role of initial upper-ocean heat content (OHC) anomalies in the SPNA in four decadal prediction systems (DPSs) exhibiting significant skill for the wintertime NAO. First, using observations, it is found that the NAO averaged in several successive winters is significantly correlated with the SPNA OHC in the November preceding the first winter.  Second, it is shown that this relationship holds also in the DPSs, and it is stronger in the systems that exhibit higher skill for the NAO itself.  Finally, we discuss the causal chain that leads from skillfully predicted SSTs to the NAO predictability via changes in low-level baroclinicity and a key positive feedback internal to the atmosphere.

Even though multi-decadal variations in the Atlantic Meridional Overturning Circulation (AMOC) may play a key role in determining respective historical variations in the SPNA OHC, no AMOC anomalies were found in the initial conditions of the hindcasts that could explain the subsequent evolution of the NAO.  Of course, this result does not preclude an important role for the AMOC in real-world NAO predictability.  Our findings advance the understanding of the mechanisms underlying decadal predictability and raise new questions regarding the role of model fidelity and ocean–NAO feedbacks in relation to the signal-to-noise problem.

How to cite: Athanasiadis, P. J., Nicolì, D., Giaquinto, D., Patrizio, C., Yeager, S., Hermanson, L., and Pohlmann, H.: The NAO decadal predictability determined by initial ocean heat content anomalies in the subpolar North Atlantic — SST gradients playing a key role., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16494, https://doi.org/10.5194/egusphere-egu26-16494, 2026.

EGU26-17142 | Posters on site | CL4.10

Initializing climate predictions using climate states from an atmosphere- ocean coupled assimilation system 

Rashed Mahmood, Shuting Yang, and Tian Tian

Initialized climate predictions are designed to align model simulated climate variability with those of observations and also aim to correct for forced model response. Significant efforts have been made in developing these climate prediction systems during the recent years with some success in predicting certain aspects of climate on annual to multi-annual timescales. However, the prediction skill on decadal timescales remains limited. Several issues have been identified with most prominent being initial shock due to different mean states of the observational data (i.e.  observationally constrained assimilations) and the model, resulting in climate drift towards the model's own attractor usually after a few months of initialization.

In this study we present results from a new initialization approach, in which the assimilation is generated by nudging both the ocean and atmospheric component of the model towards observed SST anomalies and sea level pressure respectively using the coupled model EC-Earth3. The initial evaluations suggest that the coupled ocean-atmosphere nudging results in assimilated atmospheric and ocean states that correlates better with observations both over ocean and land regions compared to ocean only nudging. The combined nudging also improves the representation of the North Atlantic Oscillation (NAO) in the assimilated data. Further assessment of different climate components (such as sea ice extent and volume) of the assimilations are ongoing. In this work we will present evaluations carried out for these two assimilations (i.e. from ocean only and coupled ocean-atmosphere nudging) and preliminary assessment of the skill of decadal predictions initialized from the combined assimilations. Furthermore we investigate the impact of the length of nudging to generate the initial state on the prediction skill on annual to decadal time scales.

How to cite: Mahmood, R., Yang, S., and Tian, T.: Initializing climate predictions using climate states from an atmosphere- ocean coupled assimilation system, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17142, https://doi.org/10.5194/egusphere-egu26-17142, 2026.

EGU26-17343 | ECS | Posters on site | CL4.10

The Pacific-North American Pattern as a Dominant Driver of Trans-Pacific Flight Time Variability 

Joon Hee Kim and Jung-Hoon Kim

Optimizing flight trajectories against upper-level jet streams is a crucial task for aviation operations. While current daily operations are efficient, with recorded flight times showing only minor deviations from theoretical optima, the modulation of jet streams by low-frequency climate variability provides a potential source of seasonal-to-decadal predictability for flight efficiency relevant to long-term strategic planning. Using optimal flight trajectory simulations based on 44 years (1979–2022) of reanalysis data, this study investigates the variability of flight times and their connection to large-scale climate modes. We identify a distinctly large variance in wintertime round-trip flight times (RFT) for Trans-Pacific routes from East Asia to the US West Coast. In contrast, North Atlantic or Hawaii–US routes exhibit low variance due to the cancellation of anti-correlated eastbound and westbound flight times, resulting in a reduced round-trip residual. Our results reveal that the Pacific-North American (PNA) pattern is the primary driver of this variability, explaining over 70% of the inter-annual RFT variance (increasing to ~80% when combined with the Western Pacific pattern). The mechanism lies in the PNA’s dipole impact on the zonal wind structure. In the positive phase, the westerlies are intensified at low latitudes and weakened at high latitudes over the North Pacific, promoting a meridional separation of optimal routes and a simultaneous reduction of eastbound and westbound flight times, whereas the negative phase induces the opposite response. Consequently, PNA phase transitions generate large variability in RFT through a coherent response of eastbound and westbound routes. This coherent feature is absent in fixed routing schemes (e.g., Great Circle Routes) or in other regions where flight trajectories cannot diverge meridionally enough to fully adapt to the dominant atmospheric anomalies. This PNA-flight time relationship remains robust across timescales, from seasonal averages to daily variations, with decreasing explanatory power as averaging periods shorten. Furthermore, the PNA pattern is also associated with the frequency of extreme delays. Our findings highlight the strong coupling between large-scale teleconnections and flight efficiency, suggesting that seamless prediction of the PNA pattern can be directly applied to risk assessment and decision-making in the aviation sector.

Acknowledgment: This work was funded by the Korea Meteorological Administration Research and Development Program under Grant (KMI2022-00310) and by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (RS-2025-24683550).

How to cite: Kim, J. H. and Kim, J.-H.: The Pacific-North American Pattern as a Dominant Driver of Trans-Pacific Flight Time Variability, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17343, https://doi.org/10.5194/egusphere-egu26-17343, 2026.

EGU26-17982 | Posters on site | CL4.10

Does insufficient oceanic resolution contribute to the signal to noise problem in seasonal forecasts? 

Bablu Sinha, Adam Blaker, Jeremy Grist, Simon Josey, and Amber Walsh

A major limitation of present seasonal prediction systems is the well-known signal to noise problem. Ensemble climate model simulations that are initialised with real world data show a remarkable degree of prediction skill for certain variables. For example, the UK Met Office GloSea5, initialised with observations in November can predict the subsequent winter North Atlantic Oscillation index with an average skill in excess of 0.6 based on the correlation of the ensemble mean simulated winter NAOI with the corresponding observed NAOI, verified from comparing more than two decades of hindcasts with observations.

The problem arises because although the correlation of the ensemble mean prediction with observations is high, the absolute magnitude of the predicted signal is low, and the ensemble mean is poorly correlated with individual ensemble members, leading to the apparent paradox that the model is better able to predict the real world than its own ensemble members. Two deleterious consequences of the signal to noise problem are that large ensembles are required to give robust skill, making seasonal forecasts expensive, and that the underprediction of the signal lessens the societal value of the forecasts.

Despite much research, the origin of the signal to noise problem remains mysterious. Here we test the hypothesis that the signal to noise problem arises at least partly because current forecast systems do not adequately represent air-sea interaction due to insufficient oceanic resolution. We run model hindcast sets using the HadGEM3 GC3.1 climate model identical in all respects except in ocean model resolution (1/4 vs 1/12 degree), evaluate differences in how well the two configurations are able to predict their own ensemble members, and attribute these to corresponding changes in air-sea interaction, including factors such as a better resolved mesoscale eddy field and more realistic boundary currents in the higher resolution configuration.

How to cite: Sinha, B., Blaker, A., Grist, J., Josey, S., and Walsh, A.: Does insufficient oceanic resolution contribute to the signal to noise problem in seasonal forecasts?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17982, https://doi.org/10.5194/egusphere-egu26-17982, 2026.

EGU26-18707 | Orals | CL4.10

How are midlatitude seasonal forecasts affected by stochastic sea ice perturbations? 

Kristian Strommen, Michael Mayer, Andrea Storto, Jonas Spaeth, and Steffen Tietsche

Reliable Arctic sea ice forecasts are important, not just for Arctic use-cases (such as determining shipping routes), but also for the potential impact that sea ice has on the midlatitude circulation. However, sea ice forecasts are often highly underdispersive, including in the IFS, the model developed and run by the European Centre for Medium-Range Weather Forecasts (ECMWF). We describe here the implementation of a stochastic parameterization scheme to the sea ice component of the IFS, and the impact it has on seasonal forecasts in the northern hemisphere midlatitudes in summer and winter. We show that sea ice ensemble spread is generally enhanced by around 10%, resulting in a more reliable forecast. We also show that the perturbations result in small but robust mean state change in Arctic air temperatures up to at least 850hPa, as a result of robust changes to the mean sea ice. A seeming consequence of this is a large increase in 500hPa geopotential (Z500) winter forecast skill over the Euro-Atlantic sector, which partially projects onto the North Atlantic Oscillation (NAO). We conclude that sea ice stochastic perturbations can be a valuable contribution to increased reliability of seasonal forecasts of the sea ice itself and can impact seasonal forecasts of the atmosphere at high and mid latitudes.

How to cite: Strommen, K., Mayer, M., Storto, A., Spaeth, J., and Tietsche, S.: How are midlatitude seasonal forecasts affected by stochastic sea ice perturbations?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18707, https://doi.org/10.5194/egusphere-egu26-18707, 2026.

EGU26-19310 | ECS | Orals | CL4.10

Tropical-extratropical cloudbands over South America in state-of-the-art seasonal forecast systems.  

Jerry B Samuel, Marcia T Zilli, and Neil C G Hart

The rainfall during the austral summer season over vast regions of South America is primarily associated with tropical-extratropical cloudbands. These northwest-southeast oriented clusters of convective clouds trigger widespread rainfall and are influenced by slowly varying tropical and subtropical sea surface temperatures. Remote teleconnections also occur through atmospheric Rossby waves at synoptic to subseasonal timescales. Therefore, to accurately forecast these high impact weather events, state-of-the-art prediction systems need to capture processes at various temporal and spatial scales. An automated cloudband detection algorithm based on outgoing longwave radiation (OLR) is used in this study to examine the ability of various seasonal prediction systems, namely, ECMWF SEAS5, UKMO GLOSEAS6, and CPTEC/INPE BAM v1.2, to forecast cloudband characteristics. We find that these systems can represent cloudband seasonality and climatology well, although biases exist. There is significant spatial variability in cloudband prediction skill; the forecast systems predict monthly cloudband statistics over Southeastern South America and parts of tropical Amazon with some skill, whereas the skill is relatively poor over the core South Atlantic convergence zone region. The spatial variability in skill appears to depend on the cloudband - El Niño Southern Oscillation relationship (ENSO). Prediction skill is relatively higher in the months when ENSO has a larger influence on monthly cloudband count. In addition, the presence of skill over South Brazil possibly indicates that the models represent the underlying Rossby wave dynamics to some extent although the absence of skill over Central and Eastern Brazil potentially suggests the need for improvement in representing these teleconnections. The skill is, however, found to decrease rapidly with an increase in lead time, which might have to do with processes at shorter time scales and intrinsic atmospheric variability as suggested by previous studies. In line with this, the composite evolution of upper-level v-wind anomalies in the lead-up to cloudband events appears to be more zonally oriented in the seasonal prediction systems compared to observation. Despite being continental scale weather regimes, differences in upper-level teleconnections indicate that predicting tropical-extratropical cloudband occurrence at seasonal timescales remains a challenge, although the intense rainfall associated with cloudbands are often more predictable than extreme rainfall occurring on non-cloudband days.

How to cite: Samuel, J. B., Zilli, M. T., and Hart, N. C. G.: Tropical-extratropical cloudbands over South America in state-of-the-art seasonal forecast systems. , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19310, https://doi.org/10.5194/egusphere-egu26-19310, 2026.

EGU26-19534 | ECS | Orals | CL4.10

Exploring the limits of multi-annual predictability for compound hot-dry extremes 

Alvise Aranyossy, Paolo De Luca, Rashed Mahmood, and Markus Donat

Hot-dry compound extremes have recently gained attention as a result of their potential destructive impacts on environments and societies. To this end, multi-annual predictions of these events could potentially offer useful information for a variety of socio-economic sectors. However, while previous studies have successfully predicted these extremes in some regions, they still struggle to capture much of the interannual variability, with most skill stemming from long-term forcings. Here, we investigate the sources of such limitations by comparing the skill of multi-annual forecasts against a perfect-model setup, using the EC-Earth3 model. While real-world predictions are initialized towards the observed state and evaluated in their ability to predict observed climate, the perfect-model predictions are initialised and assessed against a historical simulation with the same model, ensuring physical consistency between the prediction and the reference, and avoiding the uncertainties tied to the initial conditions. By comparing the perfect-model setup (PerfSet) with the real-world setup (RealFor), we assess to what extent the inconsistencies between real-world climate and the model affect the multi-annual predictability of compound hot-dry extremes.

From a skill perspective, the relative performance of PerfSet and RealFor depends on the region analysed, with neither experiment consistently outperforming the other. Residual correlation analysis, representing the contribution of initialization to forecast skill, indicates that PerfSet generally exhibits larger areas with statistically significant correlations. These regions broadly coincide with areas where PerfSet shows higher skill, suggesting a stronger influence of initialization in this experiment. Further analyses distinguish dry conditions as a key limit to predictability for both experiments, particularly where aridity is mainly dependent on precipitation variability rather than potential evapotranspiration. These results illustrate the inherent limitations of models for multi-annual predictions and highlight how the intrinsically low predictability of precipitation constrains the predictability limits for hot-dry compound extremes, whether predicting real-world observations or a controlled reference dataset.

How to cite: Aranyossy, A., De Luca, P., Mahmood, R., and Donat, M.: Exploring the limits of multi-annual predictability for compound hot-dry extremes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19534, https://doi.org/10.5194/egusphere-egu26-19534, 2026.

EGU26-20776 | ECS | Posters on site | CL4.10

Decadal Climate Risk Prediction to Inform Social Science Data Collection 

Leonie Wolf, Daniel Gotthardt, Lars Feuerlein, Henrik Wallenhorst, Achim Oberg, Jana Sillmann, and Leonard Borchert

Recent advances in climate prediction, informed by large ensemble simulations, allow estimating probabilities of future climate extreme occurrences up to a decade in advance. This offers opportunities to assess decadal climate predictions with societal impacts in mind. However, explicit assessment of the societal impacts of decadal climate extreme predictions is rare. To address this gap, we propose a framework to bridge between climate prediction sciences and rare-event social research. Following the IPCC risk framework that establishes risk as a combination of hazard, vulnerability and exposure, we construct decadal predictions of climate risks that inform the selection of regions of particular high risk for social science data collection of pre- and post- processes. Here, we demonstrate this framework with a study on predicted decadal extreme summer temperature intensifications and urban governance.

As a first step, we target a robust integration of risk assessment into our prediction analysis. We integrate decadal hazard predictions of hot summer temperature increase with social vulnerability to this predicted hazard and population density exposure data, assuming vulnerability and exposure to be static at 2020 levels. This approach leads to a decadal risk forecast that explicitely incorporates societal factors in the predicted index. For the period 2021 to 2030, we find robust prediction of relevant hot summer risk in multiple regions: Ethiopia, Northern India-Pakistan-Afghanistan, as well as Caucasia.

As a next step, we collect data on discourse and perception of climate extremes in major cities in these regions by repeatedly crawling websites from at-risk and control actors to analyze impacts of hot summers on societal field dynamics. This lays the groundwork for selection of comparable regions where climate extremes may influence social systems, enabling a more robust methodology for tracing causal impacts from the natural into the social system.

How to cite: Wolf, L., Gotthardt, D., Feuerlein, L., Wallenhorst, H., Oberg, A., Sillmann, J., and Borchert, L.: Decadal Climate Risk Prediction to Inform Social Science Data Collection, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20776, https://doi.org/10.5194/egusphere-egu26-20776, 2026.

EGU26-21421 | ECS | Orals | CL4.10

Statistical improvement of TAG Index Prediction Skill in DCPP-A Hindcast Experiments Using Deep Learning 

Jivesh Dixit, Hariprasad Kodamana, Sukumaran Sandeep, and Krishna M. AchutaRao

Reliable climate information at multi-year lead times is essential for informed decision-making and long-term planning. Such information helps policymakers and stakeholders prepare for climate-related risks and build resilience to ongoing climate variability and change.

Decadal climate variability (DCV) affects regional climate patterns all over the world on timescales of several years to decades. Skillful prediction of these modes and their impacts can support planning several years in advance. The Tropical Atlantic SST Gradient (TAG) index is one such DCV mode, characterized by differences in sea surface temperature across the tropical Atlantic Ocean. Variations in TAG strongly affect rainfall patterns, circulation, and climate extremes in surrounding regions, including parts of Africa and South America, with important socio-economic consequences. The Decadal Climate Prediction Project (DCPP), conducted under CMIP6, provides coordinated decadal hindcast and forecast experiments to study and predict such variability.

However, traditional statistical approaches often struggle to represent the complex, non-linear, and non-stationary nature of DCV modes like TAG. Deep learning (DL) methods offer a promising alternative, as they are well suited to capturing both long-term trends and shorter-term fluctuations, as well as changes in the phase of variability.

In this study, we aim to strengthen the prediction skill of the CMIP6 multi-model ensemble (MME) TAG index for lead years 1–10 using DL-based post-processing. We apply a recurrent neural network (LSTM) to correct the raw CMIP6 MME TAG forecasts. Our results indicate that DL methods have strong potential to enhance the prediction of TAG variability, particularly in terms of its trend and phase. These findings suggest that DL can serve as a valuable complementary tool to existing dynamical models, improving real-time decadal predictions and increasing confidence in operational climate forecasting systems.

How to cite: Dixit, J., Kodamana, H., Sandeep, S., and AchutaRao, K. M.: Statistical improvement of TAG Index Prediction Skill in DCPP-A Hindcast Experiments Using Deep Learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21421, https://doi.org/10.5194/egusphere-egu26-21421, 2026.

EGU26-21781 | ECS | Posters on site | CL4.10

LLM-Assisted Workflow Orchestration for Decadal Prediction Analysis 

Alexander Fischer, Gizem Ekinci, Sebastian Willmann, and Christopher Kadow

Large language models (LLMs) offer new opportunities to make climate data analysis and prediction workflows more accessible by enabling interactive, natural language–driven interactions. Recent studies have shown that LLM-based assistants can support exploratory analysis and improve reproducibility, but operational climate prediction—particularly on seasonal to decadal time scales—often involves more complex workflows. These include standardized evaluation procedures, model–observation comparisons, calibration steps, and custom post-processing, which typically require deeper technical expertise and familiarity with specialized tools and high-performance computing (HPC) environments.

In this work, we present an LLM-assisted interface designed to support decadal climate prediction analysis by orchestrating existing evaluation and post-processing tools through natural language prompts. The system allows users to initiate multi-step workflows on HPC systems, automatically generating configuration files, handling lead-time–dependent data selection, comparing predictions against observational references, and applying calibration methods. By integrating retrieval-augmented generation (RAG), the LLM is also informed by the underlying analysis code bases, enabling scientists to flexibly define, adapt and extend workflows by composing existing functions and generating lightweight custom routines.

Our results demonstrate how LLM-driven orchestration can act as a co-pilot for complex climate prediction workflows, lowering technical barriers while preserving scientific rigor. This approach supports faster iteration, greater transparency, and improved accessibility for researchers working across seasonal to decadal prediction challenges. We discuss opportunities, implications and challenges for future climate services that arise with this new way of creating and managing complex climate-scentific workflows. Likewise, we argue that natural language interfaces have the potential to reshape how scientists interact with prediction data, models, and computational infrastructure—aligning closely with the goals of current climate prediction research and applications.

How to cite: Fischer, A., Ekinci, G., Willmann, S., and Kadow, C.: LLM-Assisted Workflow Orchestration for Decadal Prediction Analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21781, https://doi.org/10.5194/egusphere-egu26-21781, 2026.

EGU26-23065 | Orals | CL4.10

Towards impact-ready decadal climate services: The promise of hybrid approaches 

Juliette Mignot, Ramdane Alkama, Bruno Castelle, Joanne Couallier, Cheikh Modou Noreyni Fal, Guillaume Gastineau, Jérôme Ogée, Elena Provenzano, Theodore Raymond, Charlotte Sakarovitch, Benjamin Sultan, and Didier Swingedouw

In the context of climate change, societal demand for actionable climate information is rapidly increasing. Climate services aim to respond to this demand by providing relevant and usable scientific information. In this framework, pluri-annual to decadal timescales are emerging as particularly critical for stakeholder decision-making. However, uncertainty at these timescales remains large at the regional scale, primarily due to the strong influence of internal climate variability. Decadal climate prediction seeks to reduce this uncertainty, yet several major challenges remain. First, current decadal prediction systems exhibit limited skill for key variables over land, such as precipitation over Europe. Second, addressing uncertainty and supporting adaptation at pluri-annual timescales requires renewed approaches to dialogue and communication with stakeholders. Here, we present a set of actions developed by our group to address these challenges. We show that the first limitation can be partly alleviated through hybrid approaches, several of which are introduced here. We also describe processes for transferring scientific results to stakeholders, illustrated through case studies notably on water management in France and agriculture in Senegal. To conclude, those on-going developments illustrate how combining advances in prediction systems with tailored communication strategies, can more effectively support adaptation decisions in a context of persistent uncertainty.

How to cite: Mignot, J., Alkama, R., Castelle, B., Couallier, J., Modou Noreyni Fal, C., Gastineau, G., Ogée, J., Provenzano, E., Raymond, T., Sakarovitch, C., Sultan, B., and Swingedouw, D.: Towards impact-ready decadal climate services: The promise of hybrid approaches, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-23065, https://doi.org/10.5194/egusphere-egu26-23065, 2026.

NP6 – Turbulence, Transport and Diffusion

EGU26-2463 | Orals | NP6.1

Relativistic MHD turbulence in hot plasmas and synchrotron polarization properties 

Luca Del Zanna, Simone Landi, and Niccolò Bucciantini

Relativistically hot plasmas are well known astrophysical sources of synchrotron emission, and the degree of linear polarization is affected by the level of turbulence in the source. Here we show, by means of a series of 3D numerical simulations, how the properties of decaying turbulence in hot plasmas depend on the magnetization of both the initial guide field and fluctuations, and how the turbulent Kolmogorov-type cascade proceeds in time. Dissipation occurs in thin, intermittent current sheets, variance anysotropy and non-Gaussian deviations appear at small scales. The computed synthetic polarization maps and degree depend on the plasma dynamics and on the angle of the line-of-sight direction with respect to the guide field. We describe how observations of these quantities may be used to infer the turbulence properties in the source.

How to cite: Del Zanna, L., Landi, S., and Bucciantini, N.: Relativistic MHD turbulence in hot plasmas and synchrotron polarization properties, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2463, https://doi.org/10.5194/egusphere-egu26-2463, 2026.

EGU26-3454 | ECS | Orals | NP6.1

Solar Wind Turbulence Spectra and Energy Injection Upstream of Mars 

Zhuxuan Zou, Yuming Wang, Zhiyong Wu, Zhenpeng Su, and Zhenguang Huang

We statistically study the power spectral density (PSD) of the magnetic field turbulence in the upstream solar wind of the Martian bow shock by investigating the data from Tianwen-1 and MAVEN during November 13 and December 31 in 2021. Their spectral indices and break frequencies are automatically identified. According to the profiles of the PSDs, we find that they could be divided into three types A, B and C. Only less than a quarter of the events exhibit characteristics similar to the 1 AU PSDs (Type A). We observe the energy injection in more than one-third of the events (Type B), and find the disappearance of the dissipation range in over one third of the PSDs (Type C), which is likely due to the dissipation occurring at higher frequencies rather than proton cyclotron resonant frequencies.

We present an in-depth study of energy injection processes associated with Type-B spectra. Singular Value Decomposition analysis reveals that the gain regions are predominantly composed of compressive wave modes. Notably, a subset of these modes is identified as relatively pure, broadband ion cyclotron waves, a feature not recognized in prior statistical surveys of proton cyclotron waves. Statistical analysis of Type-B events observed by two spacecraft reveals spatial differences: events detected by MAVEN at the quasi-parallel bow shock nose are strongly influenced by the foreshock and correlate with reflected pickup ions. In contrast, concurrent events observed by Tianwen-1 on the flank show no clear connection to the foreshock or the ambient electric field direction, suggesting a potential link to upstream processes in the southern hemisphere.

The statistical study demonstrates the complicated turbulent environment of the solar wind upstream of the Martian bow shock.

How to cite: Zou, Z., Wang, Y., Wu, Z., Su, Z., and Huang, Z.: Solar Wind Turbulence Spectra and Energy Injection Upstream of Mars, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3454, https://doi.org/10.5194/egusphere-egu26-3454, 2026.

EGU26-3808 | ECS | Orals | NP6.1

Turbulence in the terrestrial magnetosheath: space-time correlation using MMS 

Francesco Pecora, William H Matthaeus, Antonella Greco, Pablo Dmitruk, Yan Yang, Vincenzo Carbone, and Sergio Servidio

Spatiotemporal correlation of magnetic field fluctuations is investigated using the
Magnetospheric Multiscale mission in the terrestrial magnetosheath. The first observation of
the turbulence propagator emerges through analysis of more than a thousand intervals.
Results show clear features of spatial and spectral anisotropy, leading to a distinct behavior of
relaxation times in the directions parallel and perpendicular to the mean field.
The full space-time investigation of the Taylor hypothesis presents a scale-dependent
anisotropy of the magnetosheath when compared to characteristic flow propagation time and
with Eulerian estimates.
The turbulence propagator reveals that the amplitudes of the perpendicular modes decorrelate
according to sweeping or Alfvénic mechanisms. The decorrelation time of parallel modes
instead does not depend on the parallel wavenumber which could be due to resonant
interactions.
This study provides unprecedented observations into the space-time structure of turbulent
space plasmas, also giving critical constraints for theoretical and numerical models.

How to cite: Pecora, F., Matthaeus, W. H., Greco, A., Dmitruk, P., Yang, Y., Carbone, V., and Servidio, S.: Turbulence in the terrestrial magnetosheath: space-time correlation using MMS, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3808, https://doi.org/10.5194/egusphere-egu26-3808, 2026.

EGU26-3865 | ECS | Orals | NP6.1

The Nature of Turbulence at Sub-Electron Scales in the Solar Wind 

Shiladittya Mondal, Christopher Chen, and Davide Manzini

Turbulence plays an important role in the processes responsible for solar wind heating and acceleration by transferring energy to small scales where it is ultimately dissipated. Understanding turbulence dynamics at kinetic scales is therefore essential for determining how heating occurs in a weakly-collisional plasma. While much progress has been made at magnetohydrodynamic and ion scales, sub-electron scale turbulence remains poorly understood due to limited measurements beyond magnetic field fluctuations. However, Parker Solar Probe (PSP), equipped with its high-resolution instruments and unique near-Sun orbit, provides an excellent opportunity to study turbulence at such scales. In addition to the magnetic field (B), we obtain for the first time, the density (n) spectra (using spacecraft potential measurements) extending to scales smaller than the electron gyro-radius (ρe). At scales larger than ρen and B spectra exhibit similar slopes (-2.62, -2.56), indicative of Kinetic Alfvén turbulence. Below ρe, both spectra steepen, with B steepening more than n (-3.84 vs -3.28). This difference between the slopes of the two fields is consistent with turbulence becoming electrostatic in nature and the presence of an electron entropy cascade. While the n spectra has a slope close to the -10/3 prediction, the B spectra is much shallower than the expected -16/3 slope of entropy cascade. We speculate that this apparent shallowing may be due to the finite frequency resolution of the instrument and the presence of weakly damped electromagnetic fluctuations near ρe.

How to cite: Mondal, S., Chen, C., and Manzini, D.: The Nature of Turbulence at Sub-Electron Scales in the Solar Wind, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3865, https://doi.org/10.5194/egusphere-egu26-3865, 2026.

EGU26-3992 | Orals | NP6.1

Solar wind turbulence from fluid to kinetic scales: observations at 0.053 and 1 au.  

Olga Alexandrova, Amelie Fournier, Petr Hellinger, Milan Maksimovic, Andre Mangeney, and Stuart Bale

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. We show that these electron scale events are embedded in coherent structures at ion and fluid scales. The results at 1 au are compared with spectral properties and coherent structures at kinetic scales observed by Parker Solar Probe at 11.4 solar radii distance from the Sun during Encounter 19.

How to cite: Alexandrova, O., Fournier, A., Hellinger, P., Maksimovic, M., Mangeney, A., and Bale, S.: Solar wind turbulence from fluid to kinetic scales: observations at 0.053 and 1 au. , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3992, https://doi.org/10.5194/egusphere-egu26-3992, 2026.

EGU26-4983 | ECS | Orals | NP6.1 | Highlight

Direct Observations of Solar Wind Proton Energization via Nonlinear Cyclotron Resonance 

Jinghuan Li, Yuri V. Khotyaintsev, Daniel B. Graham, and Philippe Louarn

The heating of corona and solar wind remains a fundamental but unresolved problem in space and astrophysical plasma physics. Ion cyclotron waves (ICWs) have long been proposed as a potential mechanism, energizing solar wind ions through cyclotron resonance. The wave-particle energy transfer is typically evaluated using quasilinear diffusion theory, which assumes gyrotropic ion distributions and may underestimate the actual efficiency. Therefore, high-resolution measurements of three-dimensional ion velocity distribution functions are essential to capture agyrotropic signatures arising from kinetic or nonlinear effects. Here, we report Solar Orbiter observations showing that falling-tone ICWs can efficiently energize agyrotropic protons via nonlinear cyclotron resonance. These phase-bunched ions generate resonant currents that mediate substantial energy transfer, with efficiencies up to two orders of magnitude higher than previous quasilinear estimates. These findings highlight the critical role of nonlinear wave–particle interactions in solar wind heating and acceleration, which may operate more broadly across diverse plasma environments.

How to cite: Li, J., Khotyaintsev, Y. V., Graham, D. B., and Louarn, P.: Direct Observations of Solar Wind Proton Energization via Nonlinear Cyclotron Resonance, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4983, https://doi.org/10.5194/egusphere-egu26-4983, 2026.

EGU26-5000 | ECS | Orals | NP6.1

From Large-Scale Structures to Turbulence: Advancing Virtual Spacecraft Diagnostics for Space Weather Forecasting 

Giuseppe Prete, Poedts Stefaan, Zimbardo Gatetano, and Servidio Sergio

Coronal mass ejections (CMEs) are one of the main drivers of strong space weather disturbances. The interaction between CMEs and the Earth’s magnetic field can cause a wide range of phenomena and the magnetic configuration and orientation are key factors in determining the geo-effectiveness of this type of events. Modeling these events accurately is an ongoing challenge, and data-driven simulations are a valuable operational and research tool, widely used by the community.

Using the 3D data-driven MagnetoHydroDynamical (MHD) heliospheric solar wind and CME evolution model EUHFORIA (European Heliospheric FORecasting Information Asset), our aim is to model CME events that can impact the Earth. Forthcoming missions, developed by ASI (Italian Space Agency), aims to improve space weather forecasting capabilities, particularly for CMEs, solar energetic particles (SEPs), and other interplanetary disturbances.

In particular SEPs events are of huge importance for Space Weather risks. It is well established that particle acceleration at shocks is linked to the turbulence characterizing the environment in which particles are propagating. Consequently, understanding the role of turbulence is of fundamental importance for the propagation, acceleration and characterization of SEP events. To account for these processes, we aim to integrate the effects of both large-scale structures and turbulence in the simulations, either by using 3D EUHFORIA outputs or thorough 2.5 MHD simulation performed with MPI-ArmVAC, thereby enhancing the diagnostic capabilities of virtual spacecraft.

As a case study, we analyse the event of 3 November 2021, observed by both ACE and Solar Orbiter (SolO), which were nearly co-located in latitude and longitude, with a radial separation of ~22 million km. Comparing EUHFORIA simulations with in situ data from both spacecraft provides valuable insight into the new mission’s potential performance once operational.     

This study was carried out within the Space It Up project funded by the Italian Space Agency, ASI, and the Ministry of University and Research, MUR, under Contract Grant Nos. 2024-5-E.0-CUP and I53D24000060005.                                                                                                                          

How to cite: Prete, G., Stefaan, P., Gatetano, Z., and Sergio, S.: From Large-Scale Structures to Turbulence: Advancing Virtual Spacecraft Diagnostics for Space Weather Forecasting, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5000, https://doi.org/10.5194/egusphere-egu26-5000, 2026.

EGU26-5056 | Posters on site | NP6.1

Relation of the magnetic field spectral indices with plasma properties within the heliosphere 

Jana Safrankova, Zdenek Nemecek, Frantisek Nemec, and Tereza Durovcova

The power spectral densities (PSDs) of solar wind ion moments and magnetic field turbulence in the MHD range of frequencies can be fitted by a power law with the index of -5/3 and with the power index ranging from 2 to 4 at frequencies exceeding the proton gyroscale. However, this general statement has many exceptions. As examples, (i) the density spectra exhibit a clear flattening at the high-frequency part in the MHD range but a similar effect was not reported for any other quantity, (ii) the -5/3 index is a good approximation for the magnetic field at the Earth orbit but -3/2 fits the velocity spectra better, (iii) the magnetic field spectral index evolves trough the inner heliosphere, reaching -5/3 value at 0.3 AU.  

 

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, combine them with Parker Solar Probe and Solar Orbiter observations in the inner heliosphere 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, ion and/or electron beta and cross-helicity.

How to cite: Safrankova, J., Nemecek, Z., Nemec, F., and Durovcova, T.: Relation of the magnetic field spectral indices with plasma properties within the heliosphere, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5056, https://doi.org/10.5194/egusphere-egu26-5056, 2026.

EGU26-7595 | Orals | NP6.1

Sub‑ion‑scale energy‑conversion pathways in magnetosheath turbulence 

Zoltán Vörös, Owen W. Roberts, Emiliya Yordanova, Adriana Settino, Aditi Upadhyay, Sohom Roy, Rumi Nakamura, Daniel Schmid, Martin Volwerk, and Yasuhito Narita

Turbulent small‑scale dynamo action, magnetic reconnection, and kinetic instabilities in fully three‑dimensional magnetosheath turbulence must be investigated together to understand how energy is exchanged, redistributed, and dissipated in a collisionless plasma. Clarifying how these processes coexist and how they may sequence in time is essential for understanding turbulent energy transfer at sub‑ion scales. Using high‑resolution tetrahedral MMS observations in the magnetosheath, we compute a suite of diagnostics that characterize the dynamical role of velocity‑gradient structures, including field‑aligned stretching of the magnetic field, compressive motions, pressure–strain interactions, field–particle energy conversions, and pressure‑anisotropy instability measures. All quantities are derived directly from MMS time series. The measurements errors in the considered quantities are evaluated through Monte‑Carlo–based uncertainty analysis. As a working hypothesis, we examine whether regions with strong field‑aligned stretching or compression tend to coincide with magnetic‑field amplification associated with pressure‑anisotropy instabilities, conditions that may be favorable for turbulent dynamo‑like behavior. Conversely, we test whether intervals containing potentially reconnecting thin current sheets exhibit enhanced current density, elevated field particle and pressure-strain interactions and anisotropy relaxation. To explore the temporal relationships between these processes, we apply cross‑correlation analysis to the above diagnostic measures. This approach allows us to assess whether dynamo‑like amplification statistically precedes current‑sheet formation and dissipation, or whether these processes tend to overlap. Early results suggest that both ordered sequences and simultaneous occurrences are possible, reflecting the intermittent and multi‑scale nature of collisionless turbulence. The combined diagnostic and uncertainty‑quantification framework offers a possibility to evaluate the occurrence rates of magnetic‑field amplification, reconnection, and dissipation processes in collisionless space plasmas.

How to cite: Vörös, Z., Roberts, O. W., Yordanova, E., Settino, A., Upadhyay, A., Roy, S., Nakamura, R., Schmid, D., Volwerk, M., and Narita, Y.: Sub‑ion‑scale energy‑conversion pathways in magnetosheath turbulence, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7595, https://doi.org/10.5194/egusphere-egu26-7595, 2026.

Solar Orbiter observations of homogeneous turbulence at various solar wind conditions are used to estimate the power that is carried by coherent structures above a threshold across the turbulent cascade [1]. Turbulence is a potential mechanism heating the solar wind. Both wave-wave interactions and coherent structures are mechanisms that may mediate the turbulent cascade. Coherent structures have been found to be sites of dissipation.

Following the method first proposed by Bendt & Chapman (2025) [2] a threshold is determined above which fluctuations may be coherent structures. We find that the percentage of power carried by coherent structures (LIM-P) is significant, increasing with increasing frequency and maximising at ~50% just below the scale break where the inertial range transitions to the kinetic range. At distances <0.4 AU the increase of this percentage follows a roughly linear trend. Beyond 0.4 AU, there are two subranges in the inertial range. In the kinetic range, the LIM-P decreases approximately linearly with increasing frequency. We generally find more power in coherent structures in parallel than perpendicular fluctuations. Within 0.4 AU this degree of anisotropy does not vary across inertial and kinetic ranges. Beyond 0.4 AU, there is successively more power in coherent structures perpendicular than parallel fluctuations.

If coherent structures do indeed dissipate to heat the solar wind, our results, that there is significant power in coherent structures support the idea that coherent structures are important for dissipating energy of the turbulent cascade and thus solar wind heating. The trend of the LIM-P across frequencies suggests that wave-wave interactions at larger scales are systematically supplanted by coherent structures on smaller scales.

[1] Bendt & Chapman (submitted to ApJLett) Fraction of energy carried by coherent structures in the turbulent cascade in the solar wind.

[2] Bendt & Chapman (2025) Ubiquitous threshold for coherent structures in solar wind turbulence. Phys. Rev. Research doi:10.1103/PhysRevResearch.7.023176

How to cite: Bendt, A. and Chapman, S.: Evolution of power in coherent structures across scales and heliocentric distance in solar wind turbulence, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7619, https://doi.org/10.5194/egusphere-egu26-7619, 2026.

EGU26-7817 | ECS | Orals | NP6.1

Multi-channel energy conversions and heat flux transport associated with pressure-anisotropy driven instabilities for electrons in magnetosheath turbulence 

Aditi Upadhyay, Zoltán Vörös, Sohom Roy, Ida Svenningsson, Adriana Settino, Owen W. Roberts, Emiliya Yordanova, and Rumi Nakamura

Turbulence in the terrestrial magnetosheath drives rapid energy exchanges between electromagnetic fields and flows through strong intermittent compressions, shear layers, and velocity gradient structures. These concurrent and competing processes can generate temperature anisotropies and drive plasma instabilities. Yet the dynamical pathways linking velocity-gradient processes to anisotropy evolution in compressible collisionless plasmas remain poorly understood. We combine high cadence multi-point MMS measurements to quantify the pressure–strain interaction Π: ∇u (decomposed into compressible and incompressible parts), the non-ideal work J·E, and the electron heat flux q (and ∇·q, where the signal-to-noise ratio is sufficiently large) for selected turbulent magnetosheath intervals. Physically motivated thresholds (percentile-based and background relative) identify episodes of enhanced Π: ∇u, J·E, and heat flux activity. Then, the electron temperature anisotropy Te/Te, versus parallel electron plasma βe(“Brazil”) plots are obtained from the time series under investigation, with added theoretical thresholds corresponding to whistler and firehose instabilities. In this parameter space, the trajectories of the plasma, associated with the various enhanced energy conversion and transport terms, are visualized. Case studies and ensemble statistics reveal that a dominance of different channels occurs in overlapping but non-identical regions: Π: ∇u peaks are associated with rapid anisotropy excursions and compressive structures, J·E, with localized current and electromagnetic activity, and heat flux events with directed heat-transport toward whistler and firehose thresholds. This approach offers a practical pathway to quantify how turbulence and localized structures push plasma toward or beyond linear instability thresholds, with implications for modeling dissipation and wave generation in collisionless plasmas.

How to cite: Upadhyay, A., Vörös, Z., Roy, S., Svenningsson, I., Settino, A., Roberts, O. W., Yordanova, E., and Nakamura, R.: Multi-channel energy conversions and heat flux transport associated with pressure-anisotropy driven instabilities for electrons in magnetosheath turbulence, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7817, https://doi.org/10.5194/egusphere-egu26-7817, 2026.

EGU26-7850 | ECS | Orals | NP6.1

Pressure–Strain Interaction in Collisionless Plasma Turbulence: Statistics and Scale Dependence 

Yuchen Ye, Yan Yang, Shan Wang, Tulasi Parashar, Yanwen Wang, Minping Wan, and Yipeng Shi

The Pressure--Strain interaction,  - (Pα ∇ )•uα , is a fundamental diagnostic for energy conversion in collisionless space plasmas, facilitating the exchange between bulk kinetic and internal energy for both electrons (α=e) and ions (α=i) without collisional dissipation. This interaction is traditionally decomposed into two distinct physical processes: the isotropic component , associated with dilatation, and the anisotropic component Pi-D, related to deviatoric deformation.

In this study, we perform a synchronized statistical analysis of these components by integrating Particle-In-Cell (PIC) simulations with in-situ observations from the Magnetospheric Multiscale (MMS) mission. By examining probability distribution functions (PDFs) and employing coarse-graining techniques, we identify contrasting statistical signatures for and Pi-D. Our results indicate that  exhibits nearly Gaussian PDFs with kurtosis values close to a normal distribution, suggesting relatively homogeneous fluctuations across the plasma. In contrast, Pi-D displays sharply peaked, heavy-tailed PDFs, with these tails persisting even at large scales. Notably, the extreme events within the Pi-D tails are spatially correlated with coherent structures, such as current sheets and vortices.

Furthermore, scale-dependent filtering reveals that both and Pi-D are highly sensitive to the analysis scale. However, a significant divergence is observed between PIC simulations and MMS data regarding their scale-dependent behaviors, highlighting potential differences between numerical modeling and high-resolution observations. We conclude that   serves as a distributed background channel for energy exchange, while Pi-D acts as a localized, intermittent channel. These findings clarify the statistical nature of the Pressure--Strain interaction and offer critical insights into the dissipation pathways and heating mechanisms within turbulent space environments.

How to cite: Ye, Y., Yang, Y., Wang, S., Parashar, T., Wang, Y., Wan, M., and Shi, Y.: Pressure–Strain Interaction in Collisionless Plasma Turbulence: Statistics and Scale Dependence, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7850, https://doi.org/10.5194/egusphere-egu26-7850, 2026.

EGU26-7861 | Posters on site | NP6.1

Positive residual energy of magnetohydrodynamic fast-mode shocks 

Simon Good, Kalle Palmunen, Christopher Chen, Emilia Kilpua, Timo Mäkelä, Julia Ruohotie, Chaitanya Sishtla, and Juska Soljento

The difference in energy between velocity and magnetic field fluctuations in a plasma is quantified by the residual energy.  In the solar wind, residual energy is typically negative at magnetohydrodynamic (MHD) inertial scales, indicating an excess of magnetic fluctuation energy that arises from the presence of magnetically dominated structures and a turbulent cascade.  Recent observations have shown that fast-mode shock waves, in contrast, have a conspicuous positive signature – i.e. an excess of velocity fluctuation energy – in spectrograms of residual energy.  We show how the positive residual energy of super-Alfvénic (i.e. fast-mode) MHD shocks is a natural consequence of the Rankine-Hugoniot jump conditions.  The jump conditions have been used to derive an equation for the residual energy in terms of the shock angle, density compression ratio and upstream Alfvén Mach number.  Values obtained from this equation agree well with the observed residual energies of 141 interplanetary shocks.  The potential use of positive residual energy as a fast-mode shock identification signature in spacecraft data is considered, and the significance of these findings for understanding compressive fluctuations more generally in the solar wind is briefly discussed.

How to cite: Good, S., Palmunen, K., Chen, C., Kilpua, E., Mäkelä, T., Ruohotie, J., Sishtla, C., and Soljento, J.: Positive residual energy of magnetohydrodynamic fast-mode shocks, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7861, https://doi.org/10.5194/egusphere-egu26-7861, 2026.

EGU26-8023 | Posters on site | NP6.1

Anisotropies of density and magnetic field fluctuations from inertial to kinetic scales in solar wind turbulence 

Alexander Pitna, Zdenek Nemecek, Jana Safrankova, Gary Zank, Eduard Kontar, Du Toit Strauss, and Owen Wyn Roberts

Magnetic- and density-field fluctuations in the solar wind extend over a broad range of spatial and temporal scales. At inertial (MHD) scales, magnetic-field fluctuations are dominated by Alfvénic and/or 2D turbulence, while compressive magnetic fluctuations are associated with slow and fast MHD modes. Density fluctuations at these scales arise primarily from a mixture of entropic, slow-mode, and fast-mode contributions in the transition range near ion characteristic scales, the nature of these fluctuations changes as MHD descriptions break down and kinetic effects become important. At sub-ion scales, both magnetic-field and density fluctuations are governed by fully kinetic processes. Their coupling reflects the dominance of kinetic Alfvén wave like fluctuations, leading to enhanced compressibility and altered phase relationships between density and magnetic fields. Across all these regimes, density fluctuations—tightly linked to magnetic-field variability—play a key role in the scattering of radio waves from astrophysical sources both within and beyond the heliosphere, providing a powerful diagnostic of solar-wind turbulence across scales.

In this paper, we describe observations from two long solar wind intervals measured by the BMSW instrument onboard the Spektr-R spacecraft, which provides ion density measurements at a cadence of 32 ms. Because the Spektr-R magnetometer was not operational, we analyze magnetic-field measurements from the THEMIS-C and Wind spacecraft. The analysis of density fluctuations shows that at large (inertial) scales the fluctuations are nearly isotropic, while in the kinetic range they become strongly anisotropic. In contrast, magnetic-field fluctuations display pronounced anisotropy in both the inertial and kinetic ranges. We discuss the differing anisotropic properties of density and magnetic-field fluctuations and the complications they introduce in interpreting multi-spacecraft measurements.

How to cite: Pitna, A., Nemecek, Z., Safrankova, J., Zank, G., Kontar, E., Strauss, D. T., and Roberts, O. W.: Anisotropies of density and magnetic field fluctuations from inertial to kinetic scales in solar wind turbulence, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8023, https://doi.org/10.5194/egusphere-egu26-8023, 2026.

EGU26-9415 | Orals | NP6.1

Turbulence and kinetic signatures around switchbacks in the inner heliosphere 

Silvia Perri, Denise Perrone, Adriana Settino, Federica Chiappetta, Raffaella D'Amicis, Rossana De Marco, Francesco Pecora, and Roberto Bruno

Magnetic switchbacks are large-amplitude magnetic field deflections of Alfvénic nature that are characterized by a high degree of correlation between the velocity and the magnetic fields. They are routinely detected in the inner heliosphere and are characterized by timescales that vary from hundreds of seconds up to a few hours. By means of high cadence Solar Orbiter measurements for the magnetic field vector from the fluxgate magnetometer MAG and for the reprocessed ion data sampled  from the Proton and Alpha particle sensor (PAS) of the Solar Wind Analyser (SWA) suite, we have investigated their turbulent properties in terms of Alfvénicity, structure functions, and intermittency, but also how their presence affect ion kinetic features. In particular, the analysis of a case-study switchback has shown that proton and alpha particle densities increase within it, suggesting ongoing wave activity. Very interestingly, we observe a clear correlation between the magnetic deflection and alpha particle temperature, while no correlation has been found with proton temperature. This is an indication of a possible role played by switchbacks in preferentially heating heavy ions. The shapes of the proton and alphas velocity distribution functions around switchbacks will also be presented and discussed.

How to cite: Perri, S., Perrone, D., Settino, A., Chiappetta, F., D'Amicis, R., De Marco, R., Pecora, F., and Bruno, R.: Turbulence and kinetic signatures around switchbacks in the inner heliosphere, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9415, https://doi.org/10.5194/egusphere-egu26-9415, 2026.

EGU26-9840 | ECS | Posters on site | NP6.1

Comparison of intermittency in the solar wind, interplanetary coronal mass ejections and their sheath regions at 1 au 

Julia Ruohotie, Simon Good, and Emilia Kilpua

Interplanetary coronal mass ejections (ICMEs) and their sheath regions represent large-scale solar wind transients with distinct plasma properties compared to the solar wind. ICMEs are characterized by the presence of a large-scale flux rope, while sheaths are known for their turbulent and variable nature. At small scales, however, ICMEs, their sheaths, and the solar wind all show signs of magnetohydrodynamic turbulence. As a common property of turbulence, intermittency has been studied extensively in the solar wind and more recently also in ICMEs and their sheaths. Since intermittency manifests as non-Gaussian distributions of fluctuations, scale-dependent kurtosis is a commonly used measure for intermittency. Kurtosis is applied in different ways, with some studies using absolute or mean values of kurtosis to quantify the non-Gaussianity of the distributions at certain scales, while others use the slope of kurtosis to characterize how distributions evolve across scales. However, the interpretation of results can depend on the chosen kurtosis measure. We use data from the Wind spacecraft to study intermittency in the slow and fast solar wind, ICMEs, and ICME sheath regions. Kurtosis is computed from the local intermittency measure through wavelet analysis. Intermittency is measured both with mean values and slopes of kurtosis in the inertial range. Both measures indicate the least amount of intermittency in the fast solar wind, while some variation is observed in the case of the most intermittent plasma environment. In addition, we examine relationships between both intermittency measures and common plasma and turbulence properties.

How to cite: Ruohotie, J., Good, S., and Kilpua, E.: Comparison of intermittency in the solar wind, interplanetary coronal mass ejections and their sheath regions at 1 au, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9840, https://doi.org/10.5194/egusphere-egu26-9840, 2026.

EGU26-11085 | ECS | Posters on site | NP6.1

Characterization of Multiple Alfvénic Solar Wind Regimes Observed by Solar Orbiter at the October 2022 Perihelion 

Omkar Sadanand Dhamane, Raffaella D'amicis, Simone Benella, Steph Yardley, rossana De marco, Roberto Bruno, Luca Sorriso-Valvo, Daniele Telloni, Denise Perrone, Christ Owen, Philip Louarn, Stefano Livi, Anil Raghav, Kishor Kumbhar, Utkarsh Sharma, Shubham Kadam, and Urvi naik

Alfvénic fluctuations are a ubiquitous, particularly in fast streams, whereas the slow wind is typically characterized by reduced Alfvénicity and enhanced variability. However, the slow wind can display strongly Alfvénic behavior as well, with fluctuation properties comparable to those of fast streams, challenging the traditional fast–slow wind dichotomy.

In this study, we perform a comparative analysis of fast solar wind and Alfvénic slow wind during the October 2022 perihelion. In particular, we investigate the solar source and the turbulent properties of the different solar wind regimes, using plasma and magnetic field measurements from the Solar Wind Analyser (SWA) and Magnetometer (MAG) instruments onboard Solar Orbiter. We further investigate possible connections between large-scale turbulence properties and small-scale dissipation by examining the relationship between inertial-range fluctuations and magnetic-field polarization at ion scales across the spectral break. By combining in situ observations with remote-sensing data and two-step ballistic backmapping, we show that Solar Orbiter was magnetically connected to the coronal hole has a bright structure within it, indicating that the observed solar wind variability is driven by spatio-temporal changes in magnetic connectivity to coronal source. Our results show that Alfvénic slow-wind interval preserve a high degree of Alfvénicity, as evidenced by large normalized cross helicity, near kinetic–magnetic energy equipartition, low magnetic compressibility, and large-amplitude magnetic and velocity fluctuations comparable to those observed in fast Alfvénic streams, despite their lower bulk speeds and higher Coulomb collisional age. These findings pose significant challenges for solar-wind models, which must account for the persistence of strong Alfvénic turbulence in slow wind originating from nearby and evolving coronal source regions while exhibiting markedly different bulk plasma properties.

How to cite: Dhamane, O. S., D'amicis, R., Benella, S., Yardley, S., De marco, R., Bruno, R., Sorriso-Valvo, L., Telloni, D., Perrone, D., Owen, C., Louarn, P., Livi, S., Raghav, A., Kumbhar, K., Sharma, U., Kadam, S., and naik, U.: Characterization of Multiple Alfvénic Solar Wind Regimes Observed by Solar Orbiter at the October 2022 Perihelion, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11085, https://doi.org/10.5194/egusphere-egu26-11085, 2026.

EGU26-11490 | ECS | Orals | NP6.1

Correlation Between Field Rotation–Strain Balance and Turbulent Cascade Processes in 3D MHD Simulations 

Conan Liptrott, Sandra Chapman, Bogdan Hnat, and Nick Watkins

Magnetohydrodynamic (MHD) turbulence is a fundamental process in astrophysical plasmas and plays a central role in energy dissipation and particle acceleration. In this work, we use high-resolution three-dimensional MHD simulations to investigate the relationship between turbulent cascade processes and the underlying structure of the magnetic and velocity fields. We determine whether regions of enhanced energy transfer and/or dissipation correlate with regions of enhanced strain- or rotation-dominated velocity and magnetic fields.

First, we apply the filtering approach [1] to coarse-grain simulation snapshots on a given scale, obtaining spatial fields of energy transfer and dissipation. We then characterise each field as strain- or rotation-dominated using the coarse-grained tensor invariants [2,3,4], with velocity and magnetic fields treated separately. Regions of intense dissipation and energy transfer are then characterised as either strain- or rotation-dominated.  This analysis is repeated across scales from the inertial range to dissipation scales to explore the relative importance of strain- and rotation-dominated features in the turbulent cascade.

The results provide insight into the phenomenology of MHD turbulence, which will be discussed in the context of recent in situ observations.

[1] M. Germano, Turbulence: the filtering approach. Journal of Fluid Mechanics. (1992) doi:10.1017/S0022112092001733

[2] V. Quattrociocchi, G. Consolini, M. F. Marcucci, and M. Materassi, On geometrical invariants of the magnetic field gradient tensor in turbulent space plasmas: Scale variability in the inertial range, Astrophys. J. (2019) doi: 10.3847/1538-4357/ab1e47

[3] B, Hnat, S. C. Chapman, C. M. Liptrott, N. W. Watkins, Solar wind magnetohydrodynamic turbulence energy transfer rate ordered by magnetic field topology Phys. Rev. Res. (2025) doi:10.1103/9wb2-r437

[4] B, Hnat, S. C. Chapman, C. M. Liptrott, N. W. Watkins, Magnetic Topology of Actively Evolving and Passively Convecting Structures in the Turbulent Solar Wind Phys. Rev. Lett. (2021) doi:10.1103/PhysRevLett.126.125101

How to cite: Liptrott, C., Chapman, S., Hnat, B., and Watkins, N.: Correlation Between Field Rotation–Strain Balance and Turbulent Cascade Processes in 3D MHD Simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11490, https://doi.org/10.5194/egusphere-egu26-11490, 2026.

EGU26-12070 | Posters on site | NP6.1

Non-Maxwellianity of ion velocity distributions in the Earth's magnetosheath 

Louis Richard, Sergio Servidio, Ida Svenningsson, Anton V. Artemyev, Kristopher G. Klein, Emiliya Yordanova, Alexandros Chasapis, Oreste Pezzi, and Yuri V. Khotyaintsev

Collisions are nearly negligible in many space and astrophysical plasmas, allowing charged-particle velocity distribution functions (VDFs) to depart from local thermodynamic equilibrium (LTE). How collisionless plasmas relax these non-LTE distributions and convert turbulent energy into particle heating remains an open question. We investigate deviations from LTE in ion velocity distribution functions (iVDFs) within collisionless plasma turbulence using high-resolution measurements from the Magnetospheric Multiscale (MMS) mission. We find that the iVDFs' non-bi-Maxwellian features are widespread and can be significant. Their complexity increases with ion plasma beta and turbulence intensity, with pronounced high-order non-LTE features emerging during intervals of large-amplitude magnetic field fluctuations. In addition, we show that turbulence-induced magnetic curvature plays a significant role in ion scattering and contributes to the isotropization of the iVDF. These results highlight the complex interaction between turbulence and the velocity distribution of charged particles, providing new insight into the kinetic processes responsible for energy conversion in collisionless plasmas.

How to cite: Richard, L., Servidio, S., Svenningsson, I., Artemyev, A. V., Klein, K. G., Yordanova, E., Chasapis, A., Pezzi, O., and Khotyaintsev, Y. V.: Non-Maxwellianity of ion velocity distributions in the Earth's magnetosheath, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12070, https://doi.org/10.5194/egusphere-egu26-12070, 2026.

EGU26-13035 | Orals | NP6.1

Intermittency and Multifractality of Elsasser Variables in Turbulent Solar Wind 

Giuseppe Consolini, Daniele Belardinelli, Simone Benella, and Raffaella D'Amicis

A natural laboratory for studying turbulence in space plasmas is the Solar Wind. The existence of intermittency in the inertial range, where the plasma dynamics can be explained within the framework of the magnetohydrodynamic model, is one of the primary characteristics of the observed turbulence. The emergence of anomalous scaling characteristics and multifractality for both magnetic and velocity field variations is the evidence of intermittency. Here, we examine the multifractal nature of the Elsasser variables demonstrating the various intermittent degrees of z± variations using data from Solar Orbiter.  Additionally, by examining the joint-multi fractal spectrum, we investigate the relationship between the singularity spectra of z± fluctuations. In relation to the asymmetry of the observed singularity spectra, the significance of stochastic energy redistribution throughout the inertial cascade is also discussed.

This research is supported by the Space It Up! project funded by the Italian Space Agency, ASI, and the Ministry of University and Research, MUR, under contract n. 2024-5-E.0—CUP n. I53D24000060005.

How to cite: Consolini, G., Belardinelli, D., Benella, S., and D'Amicis, R.: Intermittency and Multifractality of Elsasser Variables in Turbulent Solar Wind, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13035, https://doi.org/10.5194/egusphere-egu26-13035, 2026.

EGU26-13144 | Posters on site | NP6.1

Relaxation and Coherent Structures in Space Plasma Turbulence 

Sergio Servidio, Francesco Pecora, Elisa Maria Fortugno, Antonella Greco, Mario Imbrogno, and William H. Matthaeus

In space plasmas, turbulent relaxation processes lead to the spontaneous formation of long-lived, coherent structures. By combining solar wind observations, theoretical models, and numerical simulations, we demonstrate how the plasma locally evolves toward metastable, force-free equilibria. These persistent vortices, observed within the turbulent inertial range, act as sites for particle energization and trapping, directly influencing transport and acceleration — especially in reconnection regions between interacting magnetic islands. Recent high-resolution Magnetospheric Multiscale (MMS) measurements in the magnetosheath provide direct observational evidence of such structures, confirming their central role in mediating the turbulent cascade and dissipation. This study was carried out within the Space It Up project, funded by the Italian Space Agency (ASI) and the Ministry of University and Research (MUR), under Contract Grant Nos. 2024-5-E.0-CUP and I53D24000060005.

How to cite: Servidio, S., Pecora, F., Fortugno, E. M., Greco, A., Imbrogno, M., and Matthaeus, W. H.: Relaxation and Coherent Structures in Space Plasma Turbulence, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13144, https://doi.org/10.5194/egusphere-egu26-13144, 2026.

EGU26-13712 | ECS | Orals | NP6.1

Phase-Space Dynamics of Electron Acoustic Turbulence in 2D-2V Inhomogeneous Plasmas 

Gabriele Celebre, Mario Imbrogno, Sergio Servidio, and Francesco Valentini

In weakly collisional plasmas, a complete understanding of the turbulent cascade at kinetic scales remains a fundamental and elusive problem. In this regime, spatial and velocity-space fluctuations are inherently coupled, giving rise to complex patterns in which electrostatic waves continuously interact with a network of nonlinear coherent structures. This complex interplay, potentially ubiquitous across turbulent plasma environments, is thought to play a central role in controlling energy transport and dissipation. In this research, we report the first direct investigation of the nonlinear interaction between electrostatic waves and density holes at Debye and sub-Debye scales, using high-resolution Vlasov–Poisson simulations to model the dynamics of a four-dimensional (2D–2V) plasma distribution. In particular, we construct an inhomogeneous equilibrium embedded in a proton background, consisting of a periodic lattice of electron density gaps, and perturb it with nonlinear plasma oscillations in the form of turbulent electron acoustic waves. The resulting dynamics reveal a distinctive regime in which wave–hole interaction redirects the originally one-directional, wave-driven cascade into the full phase space, uncovering a previously unexplored pathway for the emergence of phase-space structures and the transfer of energy across kinetic scales.

How to cite: Celebre, G., Imbrogno, M., Servidio, S., and Valentini, F.: Phase-Space Dynamics of Electron Acoustic Turbulence in 2D-2V Inhomogeneous Plasmas, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13712, https://doi.org/10.5194/egusphere-egu26-13712, 2026.

EGU26-14375 | Posters on site | NP6.1

Expansion and shear effects on cross-scale energy transfer rate: the SEAT model 

Victor Montagud-Camps, Andrea Verdini, Petr Hellinger, and Jaume Terradas

The energy spectrum of magnetic field fluctuations in fast and alfvénic slow solar winds generally presents a spectral break at low frequencies that separates two distinct regions. In the high-frequency side of the break, the spectrum follows a power-law in frequency with exponents that vary about -3/2 and -5/3. In the lower-frequency side of the spectral break, corresponding to the largest physical scales, the spectrum is less steep and presents a power law as the inverse of the frequency. In the same range of scales, plasma fluctuations in the heliosphere are affected by deformations of the flow due to the expansion of the solar wind and velocity shear caused by wind stream interaction. We investigate the impact of these large-scale deformations of the plasma flow on turbulence properties, with our main focus being the rate at which energy of the fluctuations is transferred from large to small scales. In our study, the energy transfer rate is estimated from a Karman-Howarth-Monin (KHM) equation, a scale-dependent energy budget equation that allows to quantify the contributions of different terms to the energy transfer. We have derived a KHM equation that accounts for the combined contribution of expansion and shear in two particular cases: when the planes affected by Shear and Expansion are Aligned or Transverse (SEAT) to each other. We will present the plasma SEAT equations that model the large-scale deformation of the plasma flow, the KHM equations derived from it and preliminary numerical results from 3D single-fluid simulations that will show how both large-scale deformation of the flow intervene in the cross-scale energy transfer and affect turbulence properties.

How to cite: Montagud-Camps, V., Verdini, A., Hellinger, P., and Terradas, J.: Expansion and shear effects on cross-scale energy transfer rate: the SEAT model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14375, https://doi.org/10.5194/egusphere-egu26-14375, 2026.

EGU26-14395 | ECS | Orals | NP6.1

Statistics of Locally Averaged Energy Transfer Rate in Plasma Turbulence 

Zihang Cheng and Yan Yang

Energy transfer across scales is essential for understanding the dissipation and heating of plasma turbulence. In the energy cascade scenario, the energy transfer rate is generally quantified by the dissipation rate in the small dissipation range, along with the third-order law in the inertial range. To investigate the local properties of the energy transfer process, here we employ three main diagnostics: the locally averaged dissipation rate  εr at different scales r, the local energy transfer (LET) rate, and the scale-filtered energy flux. The direct numerical simulation of three-dimensional incompressible magnetohydrodynamic (MHD) turbulence is conducted. Preliminary results include: (i) the spatial distributions of these energy transfer diagnostics show scale dependence, which also suggests that these diagnostics dominate at different scales; and (ii) even though these diagnostics could not be pointwise correlated, they exhibit similar patterns. To further quantify their correlation, we calculated the correlation functions, which show that the energy dissipation rate, the LET, and the scale-filtered energy flux have regional correlation, that is, they occur in close proximity to each other. Further analyses shall be conducted from several aspects: (i) taking into account the anisotropic effect on the energy transfer process, and (ii) extending into kinetic systems, wherein kinetic particle-in-cell (PIC) simulations shall be used, and the energy conversion channels, such as pressure-strain interaction and electromagnetic work, will be employed. 

How to cite: Cheng, Z. and Yang, Y.: Statistics of Locally Averaged Energy Transfer Rate in Plasma Turbulence, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14395, https://doi.org/10.5194/egusphere-egu26-14395, 2026.

EGU26-14406 | Posters on site | NP6.1

Energetic Particle Transport in Structured and Multiscale Plasma Turbulence: Bridging Observations, Theory, and Simulation 

Frederic Effenberger, Jeremiah Lübke, Horst Fichtner, and Rainer Grauer

Energetic particles in astrophysical plasmas, both in the heliosphere and in a variety of cosmic environments, interact with turbulence that is magnetised, intermittent, and inherently multiscale. Understanding how these turbulent structures govern particle transport and acceleration is key to interpreting cosmic ray propagation, space weather phenomena, and high-energy radiation signatures. Here, I report on intial results of our ISSI Team #24-608 that brings together experts in space plasma turbulence, particle transport modeling, and spacecraft data analysis to develop the next generation of physically realistic test-particle simulations. These models incorporate turbulence features constrained by heliospheric in-situ observations from Parker Solar Probe and Solar Orbiter, as well as numerical simulations resolving coherent structures like current sheets and flux ropes across broad dynamical ranges. We investigate the role of such intermittency and structure in modifying classical diffusion coefficients and enabling anomalous transport regimes. Our approach aims to move beyond idealised turbulence assumptions, providing testable predictions for particle fluxes and anisotropies in the heliosphere and beyond. These developments offer new perspectives on energetic particle dynamics across cosmic environments, with implications for galaxy-scale feedback processes and magnetised turbulence from star-forming regions to the intergalactic medium.

How to cite: Effenberger, F., Lübke, J., Fichtner, H., and Grauer, R.: Energetic Particle Transport in Structured and Multiscale Plasma Turbulence: Bridging Observations, Theory, and Simulation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14406, https://doi.org/10.5194/egusphere-egu26-14406, 2026.

We verify the level of multifractality of the solar wind magnetic field fluctuations (energy density and components) measured by the Parker Solar Probe (PSP) during its first perihelion (01-09.11.2018), recently reported in literature. Two different complementary fractal approaches, namely the Rank Ordered Multifractal Analysis (ROMA, Chang and Wu 2008) and the Partition Function Multifractal Analysis (PFMA, Halsey et al. 1986) are applied, for the first time, on the same data set. ROMA considers the raw fluctuations at all scales, grouped according to their rank; PFMA provides a multifractal spectrum from a measure extracted from data and assumed to be the result of a multiplicative process. The methodology provides new insights on the multifractality close to the Sun (at 0.17-0.23 au), and complements other studies of the same dataset, at close distances from the Sun, and at solar minimum.

At 0.17 au, a cross-over is identified at a narrow range of scales centered on ~4 s (corresponding to a spatial scale of ~1400 km) separating two sub-ranges of inertial scales, with different statistical and fractal properties. The cross-over is detected by four different approaches (1) flatness behavior, (2) structure functions power law scaling, (3) change of turbulence regime across the inertial range, (4) change of the ROMA spectra over the two inertial scale-ranges. Left-skewed asymmetry of PFMA multifractal spectra further supports the complexity of the underlying dynamics dominated by large fluctuations. Conversely, the lack of right-skewed multifractal spectra at 0.17 au, as detected in the outer heliosphere, underline the different state of fluctuations near the Sun. The results have been recently accepted for publication in the Astrophysical Journal (Teodorescu et al., 2026).

 

Chang, T., & Wu , C.C. 2008, PhRvE, 77, 045401. doi:10.1103/PhysRevE.77.045401

Halsey, T. C., Jensen, M. H., Kadanoff, L. P. et al. 1986, PhRvA, 33, 1141–1151. doi:10.1103/PhysRevA.33.1141

Teodorescu, E., Wawrzaszek, E., Echim, M., 2026, ApJ, DOI: 10.3847/1538-4357/ae3185

How to cite: Teodorescu, E., Wawrzaszek, A., and Echim, M.: Bifractality and Cross-over Behavior Observed in Solar Wind Intermittency by Parker Solar Probe: Rank Ordered Analysis and Partition Function Approach, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14470, https://doi.org/10.5194/egusphere-egu26-14470, 2026.

EGU26-16141 | ECS | Orals | NP6.1

First Laboratory Observations of Residual Energy Generation in Strong Alfvén Wave Interactions 

Mel Abler, Seth Dorfman, and Christopher HK Chen

In the MHD inertial range (scales larger than ion-kinetic scales) turbulent fluctuations in the solar wind are often Alfvénic in character, meaning that their magnetic and flow velocity fluctuations are proportional to each other and predominantly perpendicular to the background magnetic field. However, observations of the solar wind have shown that there is a significant difference in the energy in velocity fluctuations and normalized magnetic fluctuations. This difference, called the residual energy, should be zero for linear Alfvén waves, but is consistently observed to be negative in the solar wind, with magnetic fluctuations dominating. This work investigates the energy partition in strong three-wave interactions through an experimental campaign on the LArge Plasma Device (LAPD) in an MHD-like regime. Primary (driven) modes are launched from antennas, and secondary modes generated by the strong three-wave interaction are observed. The primary modes are shown to have no residual energy, while the secondary modes have significant residual energy - negative in the “sum” mode and positive in the “difference” mode. These results constitute the first laboratory demonstration that residual energy can indeed be generated by nonlinear mode coupling.

How to cite: Abler, M., Dorfman, S., and Chen, C. H.: First Laboratory Observations of Residual Energy Generation in Strong Alfvén Wave Interactions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16141, https://doi.org/10.5194/egusphere-egu26-16141, 2026.

EGU26-19459 | ECS | Orals | NP6.1

Phase space cascade in the inner Heliosphere  

Andrea Larosa, Oreste Pezzi, Domenico Trotta, Hao Ran, and Luca Sorriso-Valvo

The velocity distribution functions (VDFs) of space plasma typically present non-Maxwellian shapes due to the very low level of collisisionality. The small scale gradients of the VDFs could be the key feature to explain heating and dissipation, inibiting the revesibility of the energy exchange between fields and particles once a significant level of complexity is achieved.
In this work, we investigate the solar wind protons VDFs fine features and their relation to different measures of the real space turbulent cascade. We explore different solar wind regimes and heliocentrice distances by using both Parker Solar Probe and Solar Orbiter data.
These results, suggestive of the presence of a dual velocity-real space cascade, contribute to a better understanding of turbulence in space plasmas.

How to cite: Larosa, A., Pezzi, O., Trotta, D., Ran, H., and Sorriso-Valvo, L.: Phase space cascade in the inner Heliosphere , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19459, https://doi.org/10.5194/egusphere-egu26-19459, 2026.

EGU26-20512 | Orals | NP6.1

Effect of Turbulence Amplitude and Correlation Length on Magnetic Reconnection Dynamics in Hybrid Simulations of Collisionless Plasmas 

Luca Franci, Emanuele Papini, Daniele Del Sario, Devesh Dhole, Petr Hellinger, Simone Landi, Andrea Verdini, and Lorenzo Matteini

The interplay between turbulence and magnetic reconnection in collisionless plasmas is of great interest in many different space and astrophysical environments. Turbulence generates ion-scale current sheets (CSs) which reconnect, driving a turbulent cascade at sub-ion scales and thus providing a channel for energy dissipation. We present a collection of high-resolution 2D and 3D hybrid (kinetic ions, fluid electrons) simulations of plasma turbulence with different physical parameters to investigate how the macroscopic properties of the turbulent plasma background affect the dynamics and statistics of magnetic reconnection. We focus our analysis on the impact of two key parameters: the energy injection scale (i.e., the turbulence correlation length) and the amplitude of the initial fluctuations with respect to the ambient magnetic field (i.e., the turbulence strength). These two, combined, also determine the nonlinear time associated with the turbulent cascade. We first compare the similarity and differences in the properties and dynamics of the turbulence itself (shape and size of coherent structures in real space, spectral properties of the turbulent fluctuations, energy transfer rate) and then the changes in the properties and dynamics of the CSs undergoing reconnection (CS thickness and aspect ratio, reconnection rate). We discuss how the above properties rescale with respect to the two key parameters in the context of existing theories and models for turbulence and magnetic reconnection and the physical implications of our findings.

How to cite: Franci, L., Papini, E., Del Sario, D., Dhole, D., Hellinger, P., Landi, S., Verdini, A., and Matteini, L.: Effect of Turbulence Amplitude and Correlation Length on Magnetic Reconnection Dynamics in Hybrid Simulations of Collisionless Plasmas, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20512, https://doi.org/10.5194/egusphere-egu26-20512, 2026.

EGU26-2476 | ECS | Posters on site | NP6.3

Collision coalescence and mutual penetration of electron phase space holes 

Yue Dong and Zhigang Yuan

As a universal nonlinear structure in space plasma, electron phase space holes, also named as electrostatic solitary waves (ESWs), have a 60-year research history. An important challenge has been to reveal the microscopic evolutionary process of ESWs. Previous simulations have shown that collision coalescences determine whether several weak ESWs can evolve into a strong one. However, the simulated collision coalescence has not yet been demonstrated in observations. Here, we employ coordinated observations from the MMS multi-satellite mission to unveil two distinct evolutionary processes: collision coalescence and mutual penetration of ESWs in space plasmas. Subsequently, collision simulations reveal that the conditions for coalescence are closely linked to the ratio of the maximum capture velocity of the trapped electrons to the hole velocity, consistent with the findings of energy balance analysis based on the virial theorem and successfully explaining the observed collision coalescence and mutual penetration of ESWs. Therefore, we provide a direct observational evidence to collision coalescence and mutual penetration of ESWs for the first time.

How to cite: Dong, Y. and Yuan, Z.: Collision coalescence and mutual penetration of electron phase space holes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2476, https://doi.org/10.5194/egusphere-egu26-2476, 2026.

Alpha particles constitute the most energetic ion population in the solar wind and play an important role in turbulent energy conversion and ion-scale heating. Yet, the physical processes governing their temperature evolution, anisotropy development, and differential streaming remain incompletely understood. Using Parker Solar Probe observations and 2.5D particle-in-cell simulations, we investigate how the alpha–proton temperature ratio regulates the subsequent alpha heating efficiency and associated kinetic signatures. The observations reveal that alpha heating and anisotropy are strongly modulated by the local value of temperature ratio. The simulations reproduce these trends, showing that increasing temperature ratio lowers the growth of alpha thermal energy, anisotropy, and differential drift. These results demonstrate that the alpha heating pathway could be self-regulated by its initial thermodynamic state, with hotter alphas remaining farther from the instability threshold and experiencing less resonant energization. Our findings provide new constraints on ion-scale dissipation in the near-Sun solar wind and offer a unified interpretation of alpha-proton heating.

How to cite: Xiong, Q. and Huang, S.: Alpha Particle Heating and Anisotropy in the Solar Wind Turbulence: Insights from PSP Observations and PIC Simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4789, https://doi.org/10.5194/egusphere-egu26-4789, 2026.

EGU26-7356 | ECS | Orals | NP6.3

Influence of upstream turbulence on plasma stability at a perpendicular shock: hybrid simulations 

Laura Vuorinen, David Burgess, Domenico Trotta, and Florian Koller

Collisionless shock waves and plasma turbulence play fundamental roles in particle acceleration and energy dissipation in space plasmas. In the heliosphere, the inherently turbulent solar wind continuously interacts with planetary bow shocks and interplanetary shocks. Such pre-existing turbulence can modulate the shock front, influence particle acceleration and transport, and modify the plasma conditions and plasma stability in the vicinity of the shock. We present a novel modelling setup in which we use MHD simulations to generate turbulent fields that are dynamically input to our hybrid shock simulations. This allows us to study the interaction between realistic plasma turbulence and a shock wave. Here we report results on the influence of upstream turbulence on plasma stability against ion kinetic instabilities downstream of a perpendicular shock. We find that while turbulence can locally drive plasma towards an unstable configuration, it generally makes the downstream plasma more stable against proton cyclotron and mirror mode instabilities. We also find that a sharp low limit in βparallelTperp/Tparallel “Brazil plots”, sometimes also seen in observations, can be caused by tracks representing adiabatic evolution of plasma in magnetic islands.

How to cite: Vuorinen, L., Burgess, D., Trotta, D., and Koller, F.: Influence of upstream turbulence on plasma stability at a perpendicular shock: hybrid simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7356, https://doi.org/10.5194/egusphere-egu26-7356, 2026.

EGU26-7873 | Orals | NP6.3

Angular dependence of third-order law in anisotropic MHD  

Yan Yang, Bin Jiang, Zhuoran Gao, Francesco Pecora, Kai Gao, Cheng Li, Sean Oughton, William Matthaeus, and Minping Wan

In solar wind turbulence, the energy transfer/dissipation rate is typically estimated using MHD third-order structure functions calculated using spacecraft observations. However, the inherent anisotropy of solar wind turbulence leads to significant variations in structure functions along different observational directions, thereby affecting the accuracy of energy-dissipation rate estimation. An unresolved issue is how to optimise the selection of observation angles under limited directional sampling to improve estimation precision. We conduct a series of MHD turbulence simulations with different mean magnetic field strengths, B0. Our analysis of the third-order structure functions reveals that the global energy dissipation rate estimated around a polar angle of θ = 60 agrees reasonably with the exact one. The speciality of 60 polar angle can be understood by the Mean Value Theorem of Integrals, since the spherical integral of the polar-angle component of the divergence of Yaglom flux is zero, and this polar-angle component changes sign around 60. Existing theory on the energy flux vector as a function of the polar angle is assessed, and supports the speciality of 60 polar angle. The angular dependence of the third-order structure functions is further assessed with virtual spacecraft data analysis. The present results can be applied to measure the turbulent dissipation rates of energy in the solar wind, which are of potential importance to other areas in which turbulence takes place, such as laboratory plasmas and astrophysics.

How to cite: Yang, Y., Jiang, B., Gao, Z., Pecora, F., Gao, K., Li, C., Oughton, S., Matthaeus, W., and Wan, M.: Angular dependence of third-order law in anisotropic MHD , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7873, https://doi.org/10.5194/egusphere-egu26-7873, 2026.

EGU26-7974 | ECS | Posters on site | NP6.3

Current sheet stress balance models of bifurcated current sheet reconnection in the solar wind 

Gabriel Ho Hin Suen, Christopher Owen, and Daniel Verscharen

The current sheet stress balance conditions describe the equilibrium between magnetic stresses and plasma pressure across a thin current sheet. We build upon existing work developed in the context of magnetotail reconnection to derive a set of stress balance conditions for reconnection outflows in the solar wind, which are typically characterised by a bifurcated reconnection current sheet (RCS). Applying our framework to a symmetric bifurcated RCS model, we determine the outflow region opening angle and beam population properties, obtaining values consistent with observations of reconnection in the solar wind. We then validate our framework against observations of solar wind reconnection outflows from Solar Orbiter, highlighting one event with properties compatible with our simple symmetric model. For this event, we estimate an outflow region opening angle ranging from 3.4°-8.2°, in line with values reported in previous studies. We also reconstruct the outflow beam distribution functions and find that the predicted beam velocities and temperatures match observations well, although the densities are underestimated. Overall, our stress balance framework captures some of the key features of solar wind reconnection outflow, including current sheet bifurcation and counter-streaming beams. Future work will extend the framework to asymmetric reconnection geometries.

How to cite: Suen, G. H. H., Owen, C., and Verscharen, D.: Current sheet stress balance models of bifurcated current sheet reconnection in the solar wind, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7974, https://doi.org/10.5194/egusphere-egu26-7974, 2026.

EGU26-8006 | ECS | Orals | NP6.3

Electron Kelvin-Helmholtz Instability at Quasi-perpendicular Shocks 

Ao Guo, Quanming Lu, San Lu, Shutao Yao, Zhongwei Yang, and Xinliang Gao

Electron-scale instabilities at collisionless shocks are central to plasma dissipation and particle energization, yet their physical origin and nonlinear consequences remain poorly constrained. In this presentation, we investigate the development and impact of electron Kelvin–Helmholtz instability (EKHI) at quasi-perpendicular shocks, which reveals a new pathway for electron acceleration and electron-scale structure formation.

High-resolution particle-in-cell simulations show that intense electron velocity shear naturally forms along the shock surface due to drift motion. When the shear layer thickness approaches electron kinetic scales, it becomes unstable to EKHI. This instability is localized within the shock transition, evolves on electron timescales, and is fundamentally distinct from ion-scale KH modes commonly observed at planetary boundaries.

In the nonlinear stage, the EKHI generates coherent electron vortices embedded within the shock ramp. These vortices are accompanied by strong bipolar parallel electric fields and pronounced charge separation, which effectively generate field-aligned electron beams therein. Interestingly, we further demonstrate that EKHI between the reforming shock fronts can produce electron vortex magnetic holes, which are electron-scale coherent structures frequently observed in turbulent plasma. This indicates a possible generation mechanism for electron-scale magnetic holes in Earth's magnetosheath.

These results identify EKHI as a key mechanism linking shock-surface shear flows, electron vortices, magnetic holes, and electron energization at quasi-perpendicular shocks. This process provides a viable pre-acceleration channel for electrons and has broad implications for kinetic-scale energy conversion at collisionless shocks.

How to cite: Guo, A., Lu, Q., Lu, S., Yao, S., Yang, Z., and Gao, X.: Electron Kelvin-Helmholtz Instability at Quasi-perpendicular Shocks, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8006, https://doi.org/10.5194/egusphere-egu26-8006, 2026.

The transport of energetic particles is intimately related to the properties of plasma turbulence, a ubiquitous dynamical process that transfers energy across a broad range of spatial and temporal scales. However, the mechanisms governing the interactions between plasma turbulence and energetic particles remain incompletely understood. Here we present comprehensive observations from the upstream region of a quasi-perpendicular interplanetary (IP) shock on 2004 January 22, using data from four Cluster spacecraft to investigate the interplay between turbulence dynamics and energetic particle transport. Our observations reveal a transition in energetic proton fluxes from exponential to power-law decay with increasing distance from the IP shock. This result provides possible observational evidence of a shift in transport behavior from normal diffusion to superdiffusion. This transition correlates with an increase in the time ratio from $\tau_s/\tau_{c}<1$ to $\tau_s/\tau_{c}\gg1$, where $\tau_s$ is the proton isotropization time, and $\tau_{c}$ is the turbulence correlation time. Additionally, the frequency-wavenumber distributions of magnetic energy in the power-law decay zone indicate that energetic particles excite linear Alfvén-like harmonic waves through gyroresonance, thereby modulating the original turbulence structure. These findings provide valuable insights for future studies on the propagation and acceleration of energetic particles in turbulent astrophysical and space plasma systems.

How to cite: Zhao, S., Yan, H., and Liu, T. Z.: Observations of Turbulence and Particle Transport at Interplanetary Shocks: Transition of Transport Regimes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11082, https://doi.org/10.5194/egusphere-egu26-11082, 2026.

EGU26-11350 | ECS | Orals | NP6.3

Formation of Suprathermal Electron Tails in an Expanding, Turbulent Solar Wind: Insights from Fully Kinetic Particle-in-Cell Simulations 

Maximilien Péters de Bonhome, Fabio Bacchini, and Viviane Pierrard

As the solar wind propagates through interplanetary space, adiabatic expansion preferentially cools the plasma in the direction perpendicular to the mean magnetic field, while leaving the temperature parallel to the field largely unaffected. The combined effect of the growing temperature anisotropy and the more rapid decrease of magnetic energy relative to the parallel pressure naturally drives the plasma toward the firehose instability threshold. Concurrently, the turbulent cascade from large to small scales leads to kinetic-scale dissipation, resulting in plasma heating and the potential development of suprathermal tails in velocity distribution functions. A central open question is how turbulence-driven heating competes with expansion-induced temperature anisotropies to regulate the onset and nonlinear evolution of kinetic instabilities. In this work, we present the first fully kinetic three-dimensional particle-in-cell (PIC) simulations of an expanding-box system that includes large-scale turbulent forcing, mimicking Alfvénic fluctuations. Our simulations reveal the emergence of suprathermal tails in the electron velocity distribution functions driven by expansion, suggesting an origin in the interplay between turbulence and the firehose instability. This work aims to bridge solar wind observations and theoretical models by providing a unified, fully kinetic framework that captures the coupled effects of expansion, turbulence-driven heating, and kinetic instabilities at electron scales.

How to cite: Péters de Bonhome, M., Bacchini, F., and Pierrard, V.: Formation of Suprathermal Electron Tails in an Expanding, Turbulent Solar Wind: Insights from Fully Kinetic Particle-in-Cell Simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11350, https://doi.org/10.5194/egusphere-egu26-11350, 2026.

EGU26-11406 | Posters on site | NP6.3

Quasilinear approach of bi-Kappa distributed electrons with dynamic κ parameter. EMEC instability 

Pablo S Moya, Roberto Navarro, Marian Lazar, Peter Yoon, Rodrigo López, and Stefaan Poedts

 In recent years, significant progress has been made in the velocity-moment-based quasilinear (QL) theory of waves and instabilities in plasmas with non-equilibrium velocity distributions (VDs) of the Kappa (or κ-) type. However, the temporal variation of the parameter κ, which quantifies the presence of suprathermal particles, is not fully captured by such a QL analysis, and typically κ remains constant during plasma dynamics. We propose a new QL modeling that goes beyond the limits of a previous approach (Moya et al. 2021), realistically assuming that the quasithermal core cannot evolve independently of energetic suprathermals. The case study is done on the electron-cyclotron (EMEC) instability generated by anisotropic bi-Kappa electrons with A = T⊥/T∥ > 1 (∥, ⊥ denoting directions with respect to the background magnetic field). The parameter κ self-consistently varies through the QL equation of kurtosis (fourth-order moment) coupled with temporal variations of the temperature components, relaxing the constraint on the independence of the low-energy (core) electrons and suprathermal high-energy tails of VDs. The results refine and extend previous approaches. A clear distinction is made between regimes that lead to a decrease or an increase in the κ parameter with saturation of the instability. What predominates is a decrease in κ, i.e., an excess of suprathermalization, which energizes suprathermal electrons due to self-generated wave fluctuations. Additionally, we found that VDs can evolve towards a quasi-Maxwellian shape (as κ increases) primarily in regimes with low beta and initial kappa values ≳ 5. The relaxation of bi-Kappa electron VDs under the action of instability is only partial by reducing the temperature anisotropy, whereas the contribution of wave fluctuations generally enhances suprathermal electrons. The present results show preliminary agreement with in-situ observations in the solar wind, suggesting that the new QL model could provide a sufficiently explanatory theoretical basis for the kinetic instabilities in natural plasmas with Kappa-like distributions.

How to cite: Moya, P. S., Navarro, R., Lazar, M., Yoon, P., López, R., and Poedts, S.: Quasilinear approach of bi-Kappa distributed electrons with dynamic κ parameter. EMEC instability, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11406, https://doi.org/10.5194/egusphere-egu26-11406, 2026.

EGU26-11844 | ECS | Orals | NP6.3

Characterising Small-Scale Structures in the Turbulent Magnetosheath Using Unsupervised Machine Learning 

Paulina Quijia Pilapaña, Julia Stawarz, and Andy Smith

In collisionless plasmas, turbulence generates intermittent small-scale structures such as intense, thin current sheets, within which magnetic reconnection can occur. These structures, and reconnection in particular, are thought to play a key role in turbulence dynamics, energy dissipation, and particle energisation. The Earth’s magnetosheath, a highly turbulent region downstream of the bow shock, provides a natural laboratory for studying these nonlinear plasma processes. The Magnetospheric MultiScale (MMS) mission offers high-resolution, multi-point observations that are ideally suited to resolving small-scale structures in this environment. However, identifying and characterising such structures in spacecraft observations remains challenging due to their localised nature, complex magnetic topology, and the wide range scales involved.

We propose an unsupervised machine learning approach to systematically identify and characterise these structures, with specific emphasis on magnetic reconnection sites within turbulent plasma observations. Our method uses the Toeplitz Inverse-Covariance Clustering (TICC) algorithm, which models each cluster as a time-invariant correlation network, enabling the detection of complex patterns in turbulence. We evaluate TICC’s ability to identify reconnection events against existing datasets and interpret its clusters using the network-based feature scores. Finally, we assess the turbulence properties associated with the identified structures and the prevalence of magnetic reconnection across multiple intervals. This study aims to provide key insight into how the role of turbulent plasmas may vary across different turbulent environments.

How to cite: Quijia Pilapaña, P., Stawarz, J., and Smith, A.: Characterising Small-Scale Structures in the Turbulent Magnetosheath Using Unsupervised Machine Learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11844, https://doi.org/10.5194/egusphere-egu26-11844, 2026.

EGU26-12428 | Orals | NP6.3

Electron Neural Closure for Turbulent Magnetosheath Simulations 

George Miloshevich, Luka Vranckx, Felipe Nathan de Oliveira Lopes, Pietro Dazzi, Giuseppe Arrò, and Pierre Henri

Modelling turbulence kinetically in space remains challenging due to the multiscale nature of plasma. An alternative approach is to adopt a fluid model hierarchy and close it using a phenomenological expression or law derived from local kinetic simulations. We address this challenge by examining decaying turbulence in the near-Earth magnetosheath using fully kinetic particle-in-cell (PIC) simulations [1]. We apply machine learning techniques to extract a non-local five-moment electron-pressure-tensor closure trained on these simulations. The data are carefully split across simulations initialized with different initial conditions, while maintaining the same turbulence and temperature levels. We evaluate the learned “equation of state” using energy-channel diagnostics, with emphasis on the pressure–strain interaction (a key mediator of turbulence heating). The new global closure outperforms common local approaches (e.g., double-adiabatic [2] and MLP-type closures [3]) in reconstructing key statistics. An equation of state trained on simulations with fewer particles per cell generalises to more accurate simulations with a higher number of particles per cell and different turbulent initialisations, while using the same physical parameters. Off-diagonal terms are more challenging to predict, but performance improves with the quantity of training data.

Finally, we couple this data-driven electron closure with kinetic ion dynamics, advancing toward hybrid kinetic simulations in which electrons are represented by a neural network-based equation of state. This hybrid physics-informed machine learning framework offers a pathway to computationally efficient models with improved physical realism, potentially enabling both predictive simulations and parameter inference in heliospheric and magnetospheric applications.

[1] G. Miloshevich, L. Vranckx, F.N. de Oliveira Lopes, P. Dazzi, G. Arrò, G. Lapenta, Phys. Plasmas 33 (2026) 012901.
[2] A. Le, J. Egedal, W. Daughton, W. Fox, N. Katz, Phys. Rev. Lett. 102 (2009) 085001.
[3] B. Laperre, J. Amaya, S. Jamal, G. Lapenta, Physics of Plasmas 29 (2022) 032706.


How to cite: Miloshevich, G., Vranckx, L., de Oliveira Lopes, F. N., Dazzi, P., Arrò, G., and Henri, P.: Electron Neural Closure for Turbulent Magnetosheath Simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12428, https://doi.org/10.5194/egusphere-egu26-12428, 2026.

EGU26-12574 | Posters on site | NP6.3

Magnetic depressions in a kinetic turbulence simulation 

Francesco Pucci, Thomas Karlsson, Giuseppe Arrò, Cyril Simon-Wedlund, Luis Preisser, Giulio Ballerini, Pierre Henri, Francesco Califano, and Martin Volwerk

We present a particle-in-cell (PIC) simulation of decaying turbulence with initial conditions representative of the solar wind, in which magnetic depressions form during the nonlinear phase. We analyse the statistical properties of these structures, including size and intensity. We analyse a few of them in detail, looking at the properties of ions and electrons inside and outside them. Using virtual spacecraft, we simulate how these structures would be observed in situ by real spacecraft. We also analyse the trajectories of a few macroparticles entering these structures and undergoing trapping. We compare our simulation results with recent Solar Orbiter observations in the solar wind.

How to cite: Pucci, F., Karlsson, T., Arrò, G., Simon-Wedlund, C., Preisser, L., Ballerini, G., Henri, P., Califano, F., and Volwerk, M.: Magnetic depressions in a kinetic turbulence simulation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12574, https://doi.org/10.5194/egusphere-egu26-12574, 2026.

EGU26-14700 | Posters on site | NP6.3

Estimating errors in energy transport terms during magnetic reconnection 

Sohom Roy, Zoltán Vörös, Adriana Settino, Rumi Nakamura, Owen Roberts, Yan Yang, Riddhi Bandyopadhyay, and William H. Matthaeus

One of the key questions about magnetic reconnection is to understand how energy is partitioned between ions and electrons, especially inside the EDR and in the outflow regions. This requires studying the energy transport terms corresponding to kinetic, thermal and electromagnetic energies respectively, along with the energy conversion terms. Previous studies have shown that ion energy flux dominates close to the EDR in magnetopause reconnection, while the electron energy flux is dominant inside it. However, one must be careful while computing the energy transport terms using MMS data, since the results can be dominated by uncertainty. This is particularly true for magnetotail reconnection, where the plasma is tenuous. Here, we present a detailed analysis of the errors in these energy transport terms, and perform a comparative study between reconnection events observed in the magnetopause, magnetosheath and magnetotail regions.

How to cite: Roy, S., Vörös, Z., Settino, A., Nakamura, R., Roberts, O., Yang, Y., Bandyopadhyay, R., and Matthaeus, W. H.: Estimating errors in energy transport terms during magnetic reconnection, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14700, https://doi.org/10.5194/egusphere-egu26-14700, 2026.

EGU26-15269 | ECS | Orals | NP6.3 | Highlight

Magnetic mirroring and curvature scattering cause anomalous cosmic-ray transport 

Jeremiah Lübke, Frederic Effenberger, Mike Wilbert, Horst Fichtner, and Rainer Grauer
We study the transport of test particles in anisotropic magnetohydrodynamic turbulence. In the regime of large fluctuations, the turbulence develops coherent structures and intermittency. Coherent field line bundles can act as magnetic mirrors and localized patches with sharp field line curvature can intermittently break magnetization of test particles. We record magnetic moment variations and experienced field line curvature around pitch-angle reversals. We find that both mechanisms (magnetic mirroring and curvature scattering) govern parallel transport via pitch-angle reversals, which occur with power-law distributed waiting times and can be modeled as a Lévy walk, while classical gyro-resonance only plays a minor role. Further, perpendicular transport is either enhanced by curvature scattering in synergy with chaotically separating field lines or diminished by magnetic mirroring due to confinement in coherent field line bundles. For strongly magnetized particles, most reversal events are caused by magnetic mirroring, while curvature scattering additionally acts on particles with small pitch angles that fall in the loss cones of most magnetic mirrors. Finally, we discuss how energy-independent transport coefficients may arise in structured intermittent turbulence.

How to cite: Lübke, J., Effenberger, F., Wilbert, M., Fichtner, H., and Grauer, R.: Magnetic mirroring and curvature scattering cause anomalous cosmic-ray transport, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15269, https://doi.org/10.5194/egusphere-egu26-15269, 2026.

EGU26-19281 | ECS | Posters on site | NP6.3

On the Anomalous Contribution to the Electric Field in Turbulent Collisionless Plasmas 

Jeffersson A. Agudelo Rueda, Julia E. Stawarz, Luca Franci, Camille Granier, and Nobumitsu Yokoi

In plasma physics, one of the main obstacles to unravelling the mechanisms responsible for energy transfer between electromagnetic fields and plasma particles is the multiscale nature of plasma phenomena. In this context, plasma turbulence plays a fundamental role because it transports energy across spatial scales from the energy injection scales (large-scales) down to small-scales at which energy is dissipated. One of the key open challenges in plasma turbulence research is understanding how the small-scale turbulent dynamics couple into and influences the large-scale behaviour of the system and how that influences the energy budget and energy transport at system scales. One approach to address this challenge is to employ so-called Large Eddy Simulations, where the large scales of the system are directly simulated, and the small-scale anomalous dynamics are parameterized using Sub-Grid-Scale (SGS) models for the anomalous contributions. However, the appropriate SGS models for describing collisionless plasma systems with large scale separations remain poorly constrained.

In this work, we employ a series of Vlasov-Hybrid simulations modelling conditions similar to turbulence in Earth’s magnetosheath to characterize the anomalous contributions to the total electric field from each term in the generalized Ohm’s law for different plasma conditions. We discuss the role of anomalous (turbulent) resistivity and anomalous viscosity on the total electric field, and we show that the most relevant anomalous contribution comes from the Hall term for plasmas with low plasma beta. We provide insight on how to model SGS terms in collisionless plasmas at scales within the kinetic range where terms associated with sub-ion physics are not necessarily negligible. To do this we establish the dependence of the anomalous terms on resolved quantities such as the magnetic field, electric current density and plasma vorticity and we evaluate their contribution to the magnetic field generation. Since electric fields strongly contribute to plasma particle energization, our results are relevant for better understanding the cross-scale energy transfer and the anomalous contribution to the energy budget.

How to cite: Agudelo Rueda, J. A., Stawarz, J. E., Franci, L., Granier, C., and Yokoi, N.: On the Anomalous Contribution to the Electric Field in Turbulent Collisionless Plasmas, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19281, https://doi.org/10.5194/egusphere-egu26-19281, 2026.

EGU26-20991 | Posters on site | NP6.3

Modelling the heliospheric magnetic field through wavelet-based synthetic turbulence 

Francesco Malara, Andrea Larosa, Francesco Pucci, Oreste Pezzi, Luca Sorriso-Valvo, Federica Chiappetta, Massimo Chimenti, Giuseppe Nisticò, Silvia Perri, and Gaetano Zimbardo

We present a model of the heliospheric magnetic field that combines a large-scale Parker Spiral component with a small-scale turbulent contribution generated using a wavelet-based approach. The turbulent fluctuations are constructed to reproduce key properties of magnetic turbulence observed in the expanding solar wind, including a radially decreasing amplitude and a spatially varying correlation length. The wavelet-based method is adapted from a previously developed Cartesian model through the introduction of a new coordinate system, which ensures the correct radial scaling of the turbulence correlation length. This approach allows us to model a wider spectral range of fluctuations than is typically achievable with magnetohydrodynamic simulations, a crucial requirement for accurately describing gyroresonant scattering of energetic particles. The model is designed for future applications in studies of energetic particle transport in the heliosphere.

How to cite: Malara, F., Larosa, A., Pucci, F., Pezzi, O., Sorriso-Valvo, L., Chiappetta, F., Chimenti, M., Nisticò, G., Perri, S., and Zimbardo, G.: Modelling the heliospheric magnetic field through wavelet-based synthetic turbulence, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20991, https://doi.org/10.5194/egusphere-egu26-20991, 2026.

EGU26-21072 | ECS | Posters on site | NP6.3

Data-Driven Identification of Region-Dependent Pressure Tensor Closures in Turbulent Space Plasmas 

Felipe Nathan de Oliveira Lopes, Pietro Dazzi, George Miloshevich, and Rony Keppens

Understanding and modelling turbulence in space plasmas requires capturing kinetic effects that go beyond standard fluid closures. In the present work, we present a data-driven framework that combines unsupervised clustering and sparse equation discovery to identify effective closures in turbulent plasmas. Our primary focus is on solar-wind observations, but with possible applications to magnetospheric environments.

We use unsupervised clustering methods, more specifically k-means, to identify dynamically similar regions in both in situ spacecraft data and numerical simulations. The first part of the project is focused on numerical simulations. Clustering is performed on multidimensional feature spaces constructed from plasma moments, fields, and other pressure-tensor-related quantities, applied to either 3D or 2D simulations. The resulting clusters define coherent regions characterized by comparable kinetic activity, anisotropy, and turbulence properties.

These clustered regions serve as domains for sparse identification of nonlinear dynamics (SINDy). Particular emphasis is placed on exploring data-driven closures involving the pressure tensor, including anisotropic and nongyrotropic contributions, and understanding their role in momentum and other dynamical equations.

The framework is designed to function consistently across both in situ measurements, such as Magnetospheric Multiscale (MMS) observations, and PIC simulations, enabling direct validation and comparison. This combined approach provides a structured method for discovering interpretable, region-specific closures in turbulent space plasmas and supports the development of reduced models directly informed by observations.

How to cite: de Oliveira Lopes, F. N., Dazzi, P., Miloshevich, G., and Keppens, R.: Data-Driven Identification of Region-Dependent Pressure Tensor Closures in Turbulent Space Plasmas, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21072, https://doi.org/10.5194/egusphere-egu26-21072, 2026.

EGU26-21383 | Posters on site | NP6.3

Magnetic field fluctuations in Jupiter's middle magnetosphere on auroral field lines 

June Piasecki, Joachim Saur, Jamey Szalay, and George Clark

Jupiter has the most powerful aurora in the solar system, which is currently studied by NASA's Juno spacecraft. Observations above Jupiter's poles have shown that electrons accelerated toward Jupiter, which contribute to auroral emissions, are frequently accompanied by electrons accelerated in the opposite direction, deep into Jupiter's large magnetosphere. These energetic, bidirectional electrons often exhibit broadband energy distributions consistent with a stochastic particle acceleration mechanism. Alfvén waves, which are observed as magnetic field fluctuations, are being discussed to play an important role in the acceleration process. These waves are belived to be generated by the discontinuous radial plasma transport from Jupiter's plasma source Io to the outer magnetosphere.  We investigate magnetic field and plasma measurements in Jupiter's middle magnetosphere, where Alfvénic fluctuations have been observed, to analyze if a correlation between magnetic field fluctuations and plasma velocity fluctuations can be observed.

How to cite: Piasecki, J., Saur, J., Szalay, J., and Clark, G.: Magnetic field fluctuations in Jupiter's middle magnetosphere on auroral field lines, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21383, https://doi.org/10.5194/egusphere-egu26-21383, 2026.

EGU26-22923 | ECS | Orals | NP6.3

Turbulent fluctuations at the Correlation Scale as the Driver of Magnetic Reconnection 

Muhammad Bilal Khan, Michael A. Shay, Sean Oughton, William H. Matthaeus, Colby Haggerty, Subash Adhikari, Paul A. Cassak, Yan Yang, Riddhi Bandyopadhyay, Sohom Roy, Daniel O’Donnell, and Samuel Fordin

Magnetic reconnection plays an important role in the turbulent relaxation of space and astrophysical plasmas, such as the solar corona, solar wind, and Earth’s magnetosheath. Recent studies have shed light on the role of magnetic reconnection as an efficient energy dissipation mechanism in these large-scale turbulent systems. However, the relative role of magnetic reconnection in dissipating turbulent energy in these macroscopic systems is still not fully understood. To investigate these issues, we simulate a turbulent plasma system using magnetohydrodynamic (MHD) simulations. A large number of reconnection sites are found, and their statistical properties are quantified. The study reveals, for the first time, that the distribution of upstream reconnecting fields is strongly correlated with the distribution of global fields at the energy-containing scales. To further explore these relations in weakly collisional systems, we perform a similar analysis on kinetic Particle-in-Cell (PIC) simulations of plasma turbulence and on in situ observations of the terrestrial magnetosheath using the Magnetospheric Multiscale Mission (MMS). Notably, the key conclusions drawn from MHD simulations remain valid in both the kinetic simulations and MMS observations. These findings are expected to significantly refine theoretical estimates of reconnection rates and heating rates resulting from magnetic reconnection.

How to cite: Khan, M. B., Shay, M. A., Oughton, S., Matthaeus, W. H., Haggerty, C., Adhikari, S., Cassak, P. A., Yang, Y., Bandyopadhyay, R., Roy, S., O’Donnell, D., and Fordin, S.: Turbulent fluctuations at the Correlation Scale as the Driver of Magnetic Reconnection, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22923, https://doi.org/10.5194/egusphere-egu26-22923, 2026.

EGU26-270 | Posters on site | NP6.4

Decoding Deep Ocean Turbulence: Bottom Mixed Layer Dynamics in the South China Sea and Western Pacific 

Joanna Zhou, Pengqi Huang, Yukfo Lai, and Shuangxi Guo

Turbulence in deep ocean environments, particularly bottom mixing, plays a critical role in multiple disciplines such as regulating energy transport, sediment resuspension, and biogeochemical exchanges. Despite its importance, bottom turbulence remains one of the least understood components of oceanography, largely due to observational challenges and the inherent complexity of seabed environments. Meanwhile, the Luzon Strait, which connects the northern South China Sea and the western Pacific Ocean, is recognized as a global hotspot for internal wave generation to the South China Sea from the Pacific Ocean. Therefore, this study investigates the structure and variability of the bottom mixed layer (BML) and its associated turbulence mechanisms across the Luzon Strait. Specifically, we aim to characterize the height of the bottom mixed layer (HBML), identify dominant physical drivers of bottom turbulence mixing, and compare mixing regimes between the northen South China Sea and the western Pacific Ocean.

Between July 27 and August 22, 2022, an oceanographic survey was conducted along both sides of the Luzon Strait. A total of 23 temperature profiles were successfully collected from two sections, 10 from the western Pacific Ocean and 13 from the northern South China Sea. The results reveal significant spatial inhomogeneity in BML characteristics across the strait. Preliminary analysis reveals that HBML is modified by a distinct mechanism on either side of the strait. In the western Pacific Ocean, HBML is positively correlated with ocean depth, suggesting that deeper regions support thicker BMLs due to weaker stratification. In the norther South China Sea, HBML appears more sensitive to seabed roughness, with thicker layers observed over complex topography. A more detailed examination of turbulence intensity and mixing efficiency is planned to further investigate these mechanisms.

In summary, by comparing mixing behavior across the norther South China Sea and western Pacific Ocean, this study advances our understanding of bottom mixed layer dynamics and contributes to the development of more accurate models for ocean circulation, which is important to improve the understanding of turbulent mixing in the deep ocean.

How to cite: Zhou, J., Huang, P., Lai, Y., and Guo, S.: Decoding Deep Ocean Turbulence: Bottom Mixed Layer Dynamics in the South China Sea and Western Pacific, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-270, https://doi.org/10.5194/egusphere-egu26-270, 2026.

EGU26-290 | Orals | NP6.4

In situ observations of density currents in a small submarine canyon in the eastern mediterranean    

Roy Jaijel, Eli Biton, Yishai Weinstein, Tal Ozer, and Timor Katz

Submarine canyons are major conduits for density currents that transport water and sediment to the deep sea. To date, most in-situ studies and observations of these currents have been conducted in large submarine canyons that either incise the shelf, are adjacent to major perennial rivers, or a combination of both features. Little, if any, observational data exist from the more globally common small submarine canyons, that may be confined to the continental slope (headless) and located far offshore from smaller, ephemeral streams. In Israel- Eastern Mediterranean, submarine canyons are found only along the northern shore. These canyons are generally small (5–20 km long) and are not connected to major coastal rivers. Whether and how these canyons serve as pathways for density currents that transport sediment to the deep Levantine Basin was unknown. To address these questions, two moored stations (landers) equipped with instrument arrays were deployed at depths of 350 m and 710m along the thalweg of the “Bat-Galim” submarine canyon, offshore Haifa. The landers operated from October 2019 to June 2020 and from September 2020 to May 2021. In both deployments, winter density currents were recorded, characterized by turbid water moving rapidly down the canyon near the seabed, with velocities comparable to those reported in larger submarine canyons. During these events, sediment-laden warm and saline shelf water plunged beneath the colder, denser canyon water, leading to temperature inversions. This inversion may cause sediment lofting and upward convection through the water column once sediment settling relieves the otherwise buoyant warm water of its ballast. Mean sediment fluxes in the canyon during these deployments were extraordinarily high compared to both the adjacent shelf and the deep sea, suggesting substantial sediment transport. These results demonstrate that the Bat-Galim canyon, and likely other submarine canyons in northern Israel, serve as active pathways for annually occurring density flows. Additionally, the findings suggest a novel turbidity flow-driven mechanism for water column convection. These unique observations highlight the need for further investigation into the possibly significant role of small submarine canyons worldwide as key conduits for water and sediment transport to the deep sea, via density currents.

How to cite: Jaijel, R., Biton, E., Weinstein, Y., Ozer, T., and Katz, T.: In situ observations of density currents in a small submarine canyon in the eastern mediterranean   , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-290, https://doi.org/10.5194/egusphere-egu26-290, 2026.

Fluctuation-dissipation relation (FDR)—a well-known theorem in statistical mechanics—comes in various versions. In an early version  (Nyquist 1928, Callen and Welton, 1951), a FDR is thought to be responsible for  the emergence of dynamical equilibrium, characterized by well-defined statistics such as variances and spectra.  A later version, proposed by Kubo (1957) and  introduced to climate research by Leith (1975) and further extended by Lucarini et al. (2017),  focuses on the response of a system to an external forcing perturbation and relates this response to the system’s restoring behavior found in the absence of perturbation.  Geophysical turbulence—generated by   dissipative systems under constant external forcing  and characterized by variances and spectra conform with the given external forcing—represents fluctuations in a dynamical equilibrium. As such, it should be governed by Nyquist’s FDR. 

 

However, it is not clear how such a FDR  is related to the differential equations that govern the evolution of  turbulent flows, not mentioning the way dissipation operates and controls the statistics of turbulent flows.  The integral fluctuation-dissipation relation (IFDR) (von Storch 2026) generalizes and extends Nyquist’s FDR.  It postulates that the IFDR resides in integrals of  differential forcings that define the governing differential equations, and represents a principle that is complementary to but  distinct from these differential equations. It is complementary in the sense that turbulent flows are described not only by solutions of the differential  equations but also by statistics, such as variance and spectra, which only emerge due to  the IFDR. It is distinct in the sense that IFDR does not exist as a time rate of change and hence cannot be included in the governing differential equations. This situation is a manifestation of the fact that in a dynamical equilibrium, the differential forcing of a component x of the full state vector is effectively non-dissipative and acts as a driver of x, while dissipation of x arises from dissipative processes implemented in equations of all components that interact with x. Such a dissipation only unfolds  when the system is integrated forward in time and reaches its maximum strength for sufficiently long integration period. The IFDR is exemplified using the Lorenz 1963 model. The identification of IFDR opens a new perspective for understanding the macroscopic behaviors of turbulent flows characterized by well-defined variances and spectra.

 

von Storch 2026: https://doi.org/10.1016/j.physa.2025.131218

How to cite: von Storch, J.-S.: Integral fluctuation-dissipation relation and  turbulence as equilibrium fluctuations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2832, https://doi.org/10.5194/egusphere-egu26-2832, 2026.

EGU26-3006 | Orals | NP6.4

Wave–Mean Flow Interactions and QBO-Like Modulations in Strato-Rotational Instabilities 

Gabriel Meletti, Jezabel Curbelo, Stéphane Adibe, Stéphane Viazzo, and Uwe Harlander

The Strato-Rotational Instability (SRI) is a hydrodynamic instability, proposed as a possible mechanism for angular-momentum transport in stratified astrophysical accretion disks. It is also a laboratory analogue for rotating stratified shear flows relevant to geophysical and planetary systems, such as  atmospheric dynamics. In Taylor–Couette flows with stable density stratification in the axial direction, the SRI generates spiral patterns that propagate alternately upward and downward along the rotation axis. While such axial reversals have been observed in experiments and numerical simulations in [1, 2], their physical origin and connection to mean-flow dynamics remain to be investigated. Here, we combine numerical simulations consistent with laboratory measurements and reduced (toy) models to investigate the mechanisms driving axial spiral propagation and low-frequency modulation in SRI. Using a Radon Transform decomposition, we isolate upward- and downward-traveling spiral components and show that each exhibits a distinct, slowly varying amplitude modulation. These modulations are phase-shifted and interact through the mean flow, leading to transitions in the direction of the axial spiral propagation. The changes also lead to changes in the axial mean flow velocity. Motivated by these observations, we introduce a reduced toy model consisting of two counter-propagating, modulated wave-like spirals. Despite its simplicity, the model clearly reproduces the observed pattern transitions, demonstrating that linear superposition of individually modulated spirals is sufficient to explain the dynamics. To interpret the simultaneous occurrence of low-frequency spiral and axial mean flow modulations, we propose a quasi-biennial oscillation (QBO)–like mechanism, inspired by several dynamical similarities of the SRI reversals with the atmospheric QBO, where the wave–mean flow interactions drive periodic reversals of the zonal flow [3, 4]. Adapting this framework to rotating stratified shear flows, we derive a reduced inertial-wave model for the axial mean flow. The model predicts periodic reversals and amplitude modulation consistent with SRI observations. Our results suggest that SRI spiral reversals arise from a weak nonlinear coupling between counter-propagating inertial waves and the mean flow, providing an interpretation linking laboratory SRI to the geophysical wave–mean flow interactions.

References [1] Meletti, G., Abide, S., Viazzo, S., Krebs, A., and Harlander, U., Experiments and long-term high-performance computations on amplitude modulations of Strato-Rotational flows, Geophysical & Astro-physical Fluid Dynamics, pp. 1–25, 2020. [2] Meletti, G., Abide, S., Viazzo, S., and Harlander, U., A parameter study of strato-rotational low-frequency modulations: impacts on momentum transfer and energy distribution, Philosophical  transactions of the Royal Society A, 381, pp. 20220297, 2023. [3] Holton, J. R. & Lindzen, R. S. An updated theory for the quasi-biennial cycle of the tropical stratosphere, Journal of Atmospheric Sciences, 29(6), pp. 1076–1080, 1972. [4] Plumb, R. A. The interaction of two internal waves with the mean flow: Implications for the theory of the quasi-biennial oscillation, Journal of Atmospheric Sciences, 34(12), pp. 1847–1858, 1977.

How to cite: Meletti, G., Curbelo, J., Adibe, S., Viazzo, S., and Harlander, U.: Wave–Mean Flow Interactions and QBO-Like Modulations in Strato-Rotational Instabilities, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3006, https://doi.org/10.5194/egusphere-egu26-3006, 2026.

EGU26-3468 | Posters on site | NP6.4

Reconstructing 4D Wind Fields from Radar Observations using Machine Learning 

Vincent Joel Peterhans, Juan Miguel Urco, Devin Huyghebaert, Jorge Chau, and Victor Avsarkisov

One of the main factors characterizing the dynamics in the atmosphere is its vertical density stratification. Gravity waves propagation upwards and breaking in the middle atmosphere play an essential role in large-scale energy transport, planetary-scale circulation and the generation of stratified turbulence, manifesting in phenomena such as the cold summer mesopause in the mesosphere. Direct observation or numerical simulation of these processes with high resolution proves difficult however due to the remoteness of the region combined with horizontal scales of 10-100km and vertical scales of 10-100m that have to be resolved for a detailed analysis of the underlying stratified turbulence.

To tackle these limitations and further our knowledge on turbulence activity in the middle atmosphere, we combine the physics-informed machine learning method HYPER (Hydrodynamic Point‐wise Environment Reconstructor) with state-of-the-art radar observations from MAARSY (Middle Atmosphere Alomar Radar System) and SIMONe (Spread-spectrum Interferometric Multistatic Meteor Radar Observing Network). The method allows reconstruction of complete 4D wind fields (spatial+temporal) based on line-of-sight measurements while adhering to Navier-Stokes-based physics constraints and has been successfully deployed previously to extract winds on 10km-scales from inputs of SIMONe. 

In our work we extend the procedure to combine the input of MAARSY and SIMONe and predict complete 4D wind fields at unprecedented horizontal and vertical resolution. Using DNS of stratified turbulence with virtual radars as a validation case, we show that our improved method is able to produce accurate results in the entire prediction domain beyond the provided measurement points, while respecting the given physics constraints. Building on this, we aim to provide a first machine learning supported analysis of stratified turbulence in the mesopause region based on radar observations.

How to cite: Peterhans, V. J., Urco, J. M., Huyghebaert, D., Chau, J., and Avsarkisov, V.: Reconstructing 4D Wind Fields from Radar Observations using Machine Learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3468, https://doi.org/10.5194/egusphere-egu26-3468, 2026.

EGU26-4493 | ECS | Posters on site | NP6.4

Roughness- and buoyancy-triggered secondary flows in gravity currents  

Dongrui Han, Zhiguo He, Yakun Guo, and Ying-tien Lin

This study uses large eddy simulations with a mixture model to investigate how secondary flows (SFs) in gravity currents (GCs), which are triggered by spanwise heterogeneous roughness or unstable buoyancy convection, influence their layer structures. These processes are analogous to those governing density-driven flows in stratified river and estuary systems. We introduce a double-averaged methodology to separate the contributions of SFs and bed roughness to the spatial fluctuations within GCs. Our results show that the spanwise locations of low and high momentum paths for GCs are locked at the crests and valleys of a rough impermeable bed, respectively, while a rough permeable boundary reverses these locations. Strong Rayleigh-Taylor instabilities developing in bed pores can eliminate the roughness-triggered SFs within GCs and generate new buoyancy-driven ones with an opposite rotation. Asymmetric boundary shear creates a barrier layer of GCs that prevents the SFs from penetrating their jet region, which continuously intensifies the rolls but restricts their vertical growth. On rough impermeable beds, these SFs sustain as a coexistence of the first and second kinds, with the first kind generated by streamwise vortex stretching. On rough permeable beds, the second kind dominates as unsteady buoyancy convection breaks the skewing of the mean shear induced by the spanwise pressure gradient. In the mean flow field, energy-transfer terms related to the SFs and bed roughness alleviate and exacerbate the uneven distribution of mean kinetic energy, respectively. In the dispersive field, the SFs-related component transfers dispersive kinetic energy from the lower part of SFs to their upper part, while the bed-roughness-related one makes an inverted transfer with a relatively small contribution. In the turbulent field, transfer terms related to the SFs and bed roughness both tend to suppress the homogenization of turbulent distribution within GCs. These findings provide insight into complex flow-bed interactions relevant to component transport and mixing processes in estuaries and oceans.

How to cite: Han, D., He, Z., Guo, Y., and Lin, Y.: Roughness- and buoyancy-triggered secondary flows in gravity currents , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4493, https://doi.org/10.5194/egusphere-egu26-4493, 2026.

EGU26-5598 | ECS | Posters on site | NP6.4

Numerical investigation of the turbulent gravity wave break-up near a critical level 

Thomas Vandamme, Juan Pedro Mellado, and Victor Avsarkisov

In stratified fluids, turbulent patches can arise due to breaking internal gravity waves (GWs). One important breaking mechanism is associated with the presence of a critical level, which occurs when the phase speed of the GW matches the background flow velocity in the direction of propagation. Linear theory predicts a diverging amplitude and energy density as the wave approaches the critical level, ultimately leading to wave breaking and the eventual onset of turbulence. However, the precise physics of the turbulent state after the wave breaking and during GW dissipation have received limited attention in the past and remains less understood. This lack in research renders a challenge for the physical representation of GW breaking in contemporary weather and climate models.

To address this issue, we perform idealized direct numerical simulations (DNS) of a GW approaching its critical level and analyze the resulting turbulent flow. We present our simulation framework and investigation results regarding different background flow configurations and obtain the scaling of the turbulent kinetic energy (TKE) dissipation with the wavelength and the background buoyancy frequency. Furthermore, Reynolds number similarity as well as the generation of secondary GWs is observed. Numerical results regarding TKE dissipation are also compared to atmospheric observations. This comparison suggests that the DNS are able to represent the physics we want to address despite their idealized nature. Additionally, the observation of secondary emissions by the turbulent layer indicates that turbulent wave breaking enables tunneling of energy across the critical level, which is a phenomenon not permitted in linear theory.

How to cite: Vandamme, T., Mellado, J. P., and Avsarkisov, V.: Numerical investigation of the turbulent gravity wave break-up near a critical level, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5598, https://doi.org/10.5194/egusphere-egu26-5598, 2026.

EGU26-5778 | Posters on site | NP6.4

The structure and lifecycle of stratified mixing by shear instability in continuously forced shear flows 

Adrien Lefauve, Christopher Bassett, Daniel Plotnick, Andone Lavery, and Rocky Geyer

The energy cascade in ocean mixing caused by stratified turbulence remains poorly understood due to the wide separation of scales at very high Reynolds numbers Re. We present a new conceptual model for this cascade, grounded in high-resolution multibeam echo-sounding observations from the mouth of the Connecticut River, a shallow salt-wedge estuary with intense interfacial mixing. During flood tide, large-scale topography and hydraulics slope the pycnocline, generating interfacial shear and Kelvin-Helmholtz billows on a vertical scale of ~1-2 m. The multibeam captures instantaneous two-dimensional images that resolve the true slopes and geometry of these instabilities, revealing the structure and evolution of turbulent mixing using acoustic backscatter as a proxy for salinity microstructure dissipation. At Re ~ 10^6, we find that mixing is dominated not by the slowly evolving billow cores, which rarely overturn, but by fast, sustained turbulence within the braids that connect them, energized by baroclinic shear within their slopes. Secondary shear instabilities within the braid are predicted by two-dimensional direct numerical simulation with parameters matching the field values. Braid dissipation and mixing is quantified by scaling arguments derived from laboratory experiments in an inclined channel, and may explain why the primary billows do not overturn. This braid-dominated mixing contrasts with the core-dominated mixing seen in transient simulations at Re ~ 10^3-10^4. We conclude that high-Re mixing hotspots continuously driven by large-scale shear – including in estuaries, wind-driven surface currents, and deep overflows – operate through fundamentally different cascade physics than implied by existing low-Re paradigms.

How to cite: Lefauve, A., Bassett, C., Plotnick, D., Lavery, A., and Geyer, R.: The structure and lifecycle of stratified mixing by shear instability in continuously forced shear flows, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5778, https://doi.org/10.5194/egusphere-egu26-5778, 2026.

EGU26-6915 | Posters on site | NP6.4

Laboratory experiments of turbulent density currents and implications for near-surface CO2 rivers dispersion 

Frédéric Girault, Marie-Margot Robert, Guillaume Carazzo, Fátima Viveiros, and Catarina Silva

Highly concentrated geogenic CO2 emissions are frequently observed in volcanic and tectonic areas. Specific topographic and meteorological conditions can lead to surface accumulation in the form of buoyancy-driven “CO2 rivers.” While history records catastrophic events, such as the deadly limnic eruption of Lake Nyos in 1986, the dynamics of these CO2 rivers are not well understood. Current modeling efforts are often limited by a lack of controlled empirical data, hindering the development of robust hazard assessment and mitigation strategies. To address this issue, we simulate CO2 rivers in scaled analog laboratory experiments by turbulently injecting high-density saline water into a tank of lower-density fresh water over a rough, inclined surface. We vary the volume flow rate, slope angle, and surface roughness between experiments. We characterize the flow dynamics by measuring the front and lateral spreading velocities as a function of time. The acquired experimental datasets are then used to calibrate TWODEE, a depth-averaged, shallow-layer numerical model for buoyancy-driven flows that relies on several empirical parameters to describe entrainment. To test the new range of parameters, we apply the calibrated model to our field data on airborne concentration and surface flux of CO2 collected at the Ribeira Grande CO2 degassing zone on São Miguel, Azores, Portugal. The results validate the experimentally calibrated model and demonstrate that our refined set of model parameters significantly improves the modeling of turbulent dense-gas flows, enabling more robust predictions of the behavior of hazardous CO2 rivers in volcanically and tectonically active regions.

How to cite: Girault, F., Robert, M.-M., Carazzo, G., Viveiros, F., and Silva, C.: Laboratory experiments of turbulent density currents and implications for near-surface CO2 rivers dispersion, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6915, https://doi.org/10.5194/egusphere-egu26-6915, 2026.

EGU26-7804 | ECS | Posters on site | NP6.4

Scale-by-scale analysis of stratified turbulence using DNS and WRF simulations 

Florencia Rodriguez, Kazim Sayeed, Manuel Fossa, Nicolas Massei, and Luminita Danaila

The increase in greenhouse gas emissions from human activities are driving a continuous rise in Earth’s temperature. The atmosphere is a highly complex system: it is vertically stratified, composed of layers with distinct flow characteristics, involves energy exchanges in both horizontal and vertical directions, exhibits heterogeneous composition, and is turbulent over a wide range of spatial and temporal scales. A detailed understanding of stratified turbulence and its role in climate dynamics is therefore essential.

Climate models necessarily rely on assumptions, either by explicitly resolving large-scale dynamics while parameterizing small-scale processes, or by focusing on small-scale turbulence with simplified representations of large-scale flows. To better understand the interactions across scales, we perform a scale-by-scale analysis based on structure functions for idealized Direct Numerical Simulation (DNS) and for Weather Research and Forecasting (WRF) model outputs.

While deriving the governing equations from both DNS and WRF datasets, second-, third- and fourth-order structure functions are computed in two-dimensions. Firstly, along the z-axis for DNS and WRF, in the direction of stratification, and secondly, in the plain perpendicular to z-axis (perpendicular to the surface). Despite differences in model complexity and scales, both datasets exhibit similar statistical behavior across orders.

The two-dimensional structure functions shows: a 90° reflection symmetry when averaging over space and time, while a 180° rotational symmetry is observed when averaging over space at each time step. Furthermore, the third-order structure function reveals a direct energy cascade aligned with the mean flow direction and an inverse energy cascade in the direction perpendicular to the mean flow. These features are consistent across both datasets and are in agreement with previous experimental observations from academic flows.

Future work will focus on separating wave-like motions, such as gravity waves, from the turbulent component in DNS and WRF outputs. This decomposition will give a clearer assessment of the respective roles of waves and turbulence in scale-by-scale energy transfers, and will help the interpretation of structure function analyses in stratified atmospheric flows.

How to cite: Rodriguez, F., Sayeed, K., Fossa, M., Massei, N., and Danaila, L.: Scale-by-scale analysis of stratified turbulence using DNS and WRF simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7804, https://doi.org/10.5194/egusphere-egu26-7804, 2026.

EGU26-9841 | ECS | Posters on site | NP6.4

Optimizing a luminescence lifetime measurement technique for non-intrusive temperature imaging in laboratory flows  

Marianne Pons, Gauthier Rousseau, Bastien Carde, Sergey Borisov, Benoit Fond, and Koen Blanckaert

Gravity-driven flows are controlled by density contrasts that can be induced, among other factors, by temperature variations. In laboratory experiments, accurately measuring temperature fields is therefore helpful to better understand the mixing mechanisms governing such flows. Optical, non-intrusive techniques are particularly valuable in this context, as they allow spatially and temporally resolved measurements without disturbing the flow.

In this study, we focus on optimizing thermal field imaging obtained using temperature-sensitive lifetime of luminescent materials. The method relies on multi-exposure accumulation within a single frame using a CMOS camera on a custom-built platform that we previously demonstrated to be significantly lower in cost while maintaining precision and sampling rates compared to specialized systems [1]. Measurements can be performed directly in the fluid, using a laser sheet to illuminate dispersed luminescent particles, or at solid boundaries when the sensing materials are coated on the container walls. Despite its proven capabilities, the method has significant optimization potential through independent refinement of both exposure and illumination durations. The main purpose of this investigation is to optimize the technique by minimizing uncertainty. To achieve this, we model uncertainty to predict a theoretically optimized timing scheme and compare it to an empirically optimized scheme. Preliminary results will be presented to assess the correspondence between theoretical and empirical uncertainty minimization, with implications for practical implementation of optimized measurement protocols. The optimized method presented here was developed using YAl3(BO3)4:Cr3+, Y3Al5O12:Cr3+ or ruby but can be applied to different luminescent material with lifetime sensitive to temperature or other quantities (i.e. pH, Oxygen, CO2, etc.).

References:

[1] Rousseau, G., Pons, M., Adelerhof, H., Pellerin, N., Giesbergen, M., Carde, B., Wolf M., Blanckaert K., Borisov S. M., & Fond, B. (2025). Low-cost CMOS-based luminescence lifetime imaging with oxygen, temperature and pH sensors. Sensors and Actuators B: Chemical, 138849, https://doi.org/10.1016/j.snb.2025.138849

How to cite: Pons, M., Rousseau, G., Carde, B., Borisov, S., Fond, B., and Blanckaert, K.: Optimizing a luminescence lifetime measurement technique for non-intrusive temperature imaging in laboratory flows , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9841, https://doi.org/10.5194/egusphere-egu26-9841, 2026.

EGU26-9959 | ECS | Posters on site | NP6.4

Mesoscale Energy Transfers in Regional domains: Spectral and Physical Space diagnostics. 

Bharath Krishnan, Yanmichel Morfa Avalos, Christoph Zülicke, and Claudia Stephan

Observations and numerical simulations consistently show that the horizontal kinetic energy spectrum follows a -5/3 slope at mesoscales from the troposphere to the lower stratosphere. Various fundamentally different theories have been proposed to explain this mesoscale spectral slope, including gravity waves, stratified turbulence, and wave-vortex interactions. To investigate the underlying mesoscale mechanism, we implement a combined diagnostic framework consisting of two complementary approaches: a non-hydrostatic, Fourier-based spectral energy budget and a scale-dependent energy transfer in physical space, used to diagnose the instantaneous, local structure of energy transfers in regional atmospheric domains, with particular emphasis on the mesosphere and lower thermosphere (MLT).

The methodology is validated using idealized mountain-wave simulations, where the dominant dynamical mechanisms are well understood. The framework is then applied to high-resolution nested UA-ICON simulations from the NASA Vorticity Experiment (VortEx) over Andøya, Norway, a dynamically active region. The results reveal pronounced spatial and scale-dependent variability in energy transfers that is not captured by domain-averaged spectral diagnostics alone. The scale-dependent energy transfers are consistent with independent turbulence indicators, including the Richardson number and parameterized turbulent kinetic energy (TKE). Regions characterized by low Richardson numbers and elevated TKE exhibit significantly stronger downscale energy cascades than those in more stable, high Richardson number regimes. This study provides insight into mesoscale dynamics by extending energy transfer analyses into the MLT and offers a robust framework for investigating energy transfer across different atmospheric regimes.

How to cite: Krishnan, B., Morfa Avalos, Y., Zülicke, C., and Stephan, C.: Mesoscale Energy Transfers in Regional domains: Spectral and Physical Space diagnostics., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9959, https://doi.org/10.5194/egusphere-egu26-9959, 2026.

EGU26-13310 | Posters on site | NP6.4

Mixing in gravity currents over an array of cylindrical obstacles 

Claudia Adduce, Maria 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 the bottom of the tank spanning its entire width. The gravity current was reproduced using the lock-release technique with a density difference ∆ρ=6 kg/m³. A total of 15 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. High-resolution density measurements reveal that the submergence ratio plays a critical role in controlling current diversion, while obstacle spacing governs the flow pathway. An increase in the submergence ratio enhances the interactions between the current and the roughness elements, resulting in marked fluctuations in potential energy and mixing intensity that significantly affect the current evolution. Although bottom roughness generally reduces the front velocity and alters entrainment behavior, the effect of obstacle spacing is less important, particularly for low submergence ratio. For large submergence ratio, the current exhibits a shift in mixing dynamics, deviating from the near-linear growth of background potential energy observed in smoother cases.

How to cite: Adduce, C., Maggi, M., and Di Lollo, G.: Mixing in gravity currents over an array of cylindrical obstacles, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13310, https://doi.org/10.5194/egusphere-egu26-13310, 2026.

EGU26-13374 | ECS | Posters on site | NP6.4

A GPU based model for multi-layer scalar transport in open channels 

Laure Sicard, Pilar Garcia Navarro, Sergio Martinez Aranda, and Borja Latorre

Scalar transport models derived from the two-dimensional depth averaged shallow water equations are frequently applied to a wide range of environmental flow conditions. A scalar may represent a dissolved solute, a pollutant, or fine sediment transported in river channels, estuaries, or ocean waters. However, these depth-averaged scalar transport models do not provide detailed information about the vertical distribution of the solute. The vertical distribution of a scalar could be computed from the 3D shallow water equations but is complex to compute numerically. One possible approach is to implement a multi-layer transport system, in which exchanges between layers determine the vertical concentration distribution of the transported scalar depending on the velocity of deposition, vertical eddy viscosity, and flow velocity.

The model presented is a GPU-based multi-layer scalar transport model implemented in C++/CUDA and coupled with an existing two-dimensional shallow water (SWE-2D) model. The SWE-2D framework is designed to handle three types of mesh topology: structured quadrilateral meshes, structured triangular meshes, and unstructured triangular meshes. The multi-layer system is implemented using an implicit scheme that accounts for interlayer exchanges. The layers are uniformly distributed in the vertical direction, with the total water depth divided by the number of layers, however, layer thickness varies in time and space with the water depth. Flux exchanges between layers depend on the vertical eddy viscosity, flow velocity, and the scalar deposition (settling) velocity. Different types of vertical eddy viscosity models have been developed (linear and constant), and the vertical flow velocity model implemented is a simple logarithmic wall low model.

To assess the viability of the multi-layer model, a series of synthetic channel test cases are implemented, in which the vertical eddy viscosity and the settling velocity are systematically varied but the vertical velocity considered as constant in depth. In addition, an experimental study by García J.A, Latorre B. et al., investigating the vertical concentration distribution of a passive solute in unsteady laboratory channel flow, is reproduced using the multi-layer framework. Results from the laboratory experiments and the numerical model are first compared using depth-averaged concentrations and, secondly, using the multi-layer system with a depth-varying vertical velocity profile. The model demonstrates a good representation of the horizontal solute distribution. Vertically, when the flow velocity varies with depth, the multi-layer system captures the solute global distribution, however , the lack of precision is due to the flow velocity and eddy viscosity vertical models that must be adapted to the specific flow conditions and environmental context.

How to cite: Sicard, L., Garcia Navarro, P., Martinez Aranda, S., and Latorre, B.: A GPU based model for multi-layer scalar transport in open channels, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13374, https://doi.org/10.5194/egusphere-egu26-13374, 2026.

EGU26-13923 | Orals | NP6.4

Backscatter in stratified turbulence 

Michael Waite and Jensen Lawrence

Kinetic energy exchanges between resolved and sub-grid motions in geophysical turbulence simulations can act in both directions: downscale transfer contributes to dissipation of the resolved kinetic energy, while upscale transfer, known as backscatter, can energize the resolved scales. Backscatter can be significant in real turbulence but is not included in many sub-grid models. This talk will discuss properties and modelling of backscatter in numerical simulations of decaying homogeneous stratified turbulence. In direct numerical simulations (DNS), we measure backscatter by filtering the solution and explicitly calculating the sub-filter energy transfers. In large eddy simulations, we include backscatter following the Leith stochastic backscatter model along with Smagorinsky eddy viscosity. Different values of the Leith coefficient are considered, and the modelled backscatter is compared to that measured in the DNS. Overall, the Leith model is capable of generating realistic levels of backscatter if the Leith coefficient is not too large. Strong backscatter forcing also changes the resolved turbulent energy transfer and leads to a reduction of kinetic energy in the inertial range. Dependence on stratification will also be discussed.

How to cite: Waite, M. and Lawrence, J.: Backscatter in stratified turbulence, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13923, https://doi.org/10.5194/egusphere-egu26-13923, 2026.

EGU26-14489 | Orals | NP6.4

The three-dimensional turbulent structure of steady state gravity currents 

Gareth Keevil, Caroline Marshall, Ed Keavney, Jeff Peakall, and Dave Hodgson

The structure of gravity currents has been extensively studied using both laboratory and numerical methods. Much of the previous work has focused on lock-exchange type flows that typically result in an exaggerated current head and a distorted turbulence distribution. The work presented herein investigates steady state gravity currents; in most natural flows the body of the flow forms the majority of the current. This study aims to quantify the three-dimensional turbulent structure of steady state gravity currents.

 

A combination of planar particle imaging velocity (PIV), shake-the-box particle tracking (StB) and acoustic measurements were used to investigate the body of pseudo-steady gravity currents, focusing on the turbulence structure and formation of coherent turbulent structures. These structures are of interest due to their ability to control the distribution of mass, momentum and temperature, as well as their potential impact on erosion and deposition in particle laden flows. PIV was used to investigate a range of Reynolds numbers by considering various slopes with a constant influx, as well as a constant slope with varying influx. StB was used to provide 3D characterisation of single Reynolds number flow in the same geometry as the PIV study. Acoustic measurements were used to quantify a number of unconfined gravity currents with a range of topographical controls.

 

The StB data describes experimentally the three-dimensional turbulent structure of the body of pseudo-steady gravity current flow for the first time. The data reveals the complex three-dimensional flow and internal waves present within gravity currents from a simple ducted domain. The results show that cross-stream and vertical flow velocities within these currents are of very similar magnitude. The unconfined study reveals the presence of significant complexity within gravity currents partially bounded by topography providing insights into the formation and spatial distribution of distinctive bedforms, such as hummock-like and sigmoidal bedforms, sediment dispersal pattern, and process controls on onlap termination styles.

How to cite: Keevil, G., Marshall, C., Keavney, E., Peakall, J., and Hodgson, D.: The three-dimensional turbulent structure of steady state gravity currents, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14489, https://doi.org/10.5194/egusphere-egu26-14489, 2026.

EGU26-15439 | ECS | Posters on site | NP6.4

Dynamics of Subglacial Plumes and Seawater Intrusion at the Ice-Ocean Interface 

Tim Redel, María Magdalena Barros, and Cristian Escauriaza

Accurate quantification of melt rates of marine-terminating glaciers is one of the most critical challenges in contemporary glaciology (Straneo & Cenedese, 2015), where small-scale ice-ocean interactions play an important role (Mamer et al., 2024). However, large-scale coupled models often misrepresent the processes that mediate these interactions, which increases uncertainty in future projections. These systems discharge substantial volumes of cold freshwater into the open ocean through subglacial plumes. The dynamics of these buoyant plumes are crucial for heat transfer, mixing, and melting processes at the ice-ocean boundary.  Previous studies have demonstrated that, under specific conditions influenced by discharge, system density, and ambient turbulence, seawater may enter the subglacial cavity as a wedge-shaped density front (Wilson et al., 2020). The mechanisms that promote or inhibit seawater intrusion and mixing remain poorly understood. To address this, we carried out direct numerical simulations (DNS) of a subglacial channel discharging into the open ocean, following the laboratory experiments of Wilson et al. (2020), and evaluated the impact of different densimetric Froude numbers on seawater intrusion and the resulting buoyant plume. Our findings provide new insights into the role of subglacial plumes in heat and salt transport, thereby clarifying the mechanisms that drive melting at the ice-ocean interface.

How to cite: Redel, T., Barros, M. M., and Escauriaza, C.: Dynamics of Subglacial Plumes and Seawater Intrusion at the Ice-Ocean Interface, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15439, https://doi.org/10.5194/egusphere-egu26-15439, 2026.

EGU26-15874 | Orals | NP6.4

Dynamics, Mixing, and Sediment Transport in the Near -Field of Freshwater Plumes 

Cristian Escauriaza, Megan Williams, and Oliver Fringer

Freshwater plumes generated by small rivers play a signficant role in coastal processes. In glacially fed systems, such as those found in Patagonia, strong buoyancy forcing and  turbulence produce sharp density interfaces and complex flow structures that regulate plume spreading and vertical exchange. Understanding the physical mechanisms controlling mixing and sediment transport in these environments is essential for linking small-scale turbulence to larger-scale coastal processes.
We present results from direct numerical simulations (DNS) of freshwater plumes discharging into denser ambient fluid under subcritical and supercritical conditions. The simulations resolve the 3D coherent structures, capturing the development of interfacial instabilities and vortical motions that control entrainment and mixing efficiency. We show that plume dynamics transition between regimes dominated by shear-driven instabilities and large-scale overturning, with distinct implications for vertical density fluxes and plume thickness.
We also explore the influence of suspended sediment on plume dynamics, focusing on how particle settling modifies turbulence, alters effective vertical transport, and feeds back on interfacial structure. The interactions of sediment transport with stratified turbulence significantly affect near-field plume evolution. These results provide new physical insights into mixing and transport in buoyancy-driven flows and help bridge idealized turbulence studies with the behavior of natural glacial river plumes in coastal environments.

This work has been supported by ONR-Global grant N62909-23-1-2004.

How to cite: Escauriaza, C., Williams, M., and Fringer, O.: Dynamics, Mixing, and Sediment Transport in the Near -Field of Freshwater Plumes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15874, https://doi.org/10.5194/egusphere-egu26-15874, 2026.

EGU26-16697 | ECS | Posters on site | NP6.4

A Multi-Scale Theory for Gravity-Wave Interaction with Turbulence 

Devadharsini Suresh, Irmgard Knop, Stamen Dolaptchiev, Rupert Klein, and Ulrich Achatz

The interaction between small-scale waves and a larger-scale flow can be described by a multi-scale theory that forms the basis for parameterizations of subgrid-scale gravity waves (GWs) in weather and climate models (e.g., Achatz et al., 2023). These parameterizations have recently been extended to include transient GW–mean-flow interactions and oblique GW propagation. Existing gravity-wave parameterizations include only rudimentary descriptions of the coupling between the dynamics of unresolved GWs and turbulence, but recent studies (Banerjee et al., 2025) have shown that this interaction is non-negligible. Energetic consistency therefore necessitates an extension of the multi-scale theory to include a more accurate representation of this interaction.

We propose an extension of this multi-scale theory that incorporates an additional turbulence formulation, allowing for a more robust bidirectional coupling between GWs and turbulence. Key results include a well-defined organization of turbulence along the phase structure of individual GWs and a correspondingly structured feedback on turbulent GW damping. We plan to present initial results from the validation of this extended theory by comparing idealized simulations with parameterized GWs to wave-resolving reference simulations.

How to cite: Suresh, D., Knop, I., Dolaptchiev, S., Klein, R., and Achatz, U.: A Multi-Scale Theory for Gravity-Wave Interaction with Turbulence, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16697, https://doi.org/10.5194/egusphere-egu26-16697, 2026.

EGU26-18700 | Orals | NP6.4

A Stratification-Dependent, Enstrophy-Controlled Regime in Baroclinic Turbulence Experiments in the Laboratory 

Peter Read, Shanshan Ding, Hadrien Bobas, Hélène Scolan, and Roland Young

The circulation of the Earth’s atmosphere and those of many other planets is dominated by turbulent interactions in a baroclinically unstable, rotating, stratified flow. Even for the Earth, which has been well observed for many years, the energy spectrum and complex properties of the anisotropic and inhomogeneous turbulent cascades of energy and enstrophy remain poorly understood and difficult to model accurately. Here we measure geostrophic turbulence energised by baroclinic instability in a rotating, differentially heated fluid annulus in the laboratory, which is bounded by convectively-driven warm and cold flows at the outer and inner boundaries, respectively (see Fig. 1a). Horizontal velocity fields (Fig. 1b-c) are obtained via particle image velocimetry of neutrally buoyant particles suspended in the flow, while the temperature structure is sampled using a vertical array of thermocouples located in the middle of the channel. The horizontal kinetic energy spectra exhibit a wavenumber range at relatively large length scales which scales as k−3, where k denotes the horizontal wavenumber (see Fig. 1d-e). Moreover, the spectral amplitude is found to correlate with the square of the Brunt–Vaisala frequency N at the same heights as the velocity measurements. The observed turbulent state exhibits a net forward enstrophy cascade across all scales, along with bidirectional kinetic energy transfer, which is indicated by a reversal in the sign of the spectral energy flux. The change of sign of the kinetic energy cascade occurs at a scale proportional to the internal Rossby radius of deformation Ld. These findings highlight the role of baroclinic instability in shaping the distribution of energy across scales with implications for synoptic- and meso-scale turbulent flows in the atmospheres of the Earth and other terrestrial planet atmospheres and oceans.

FIG. 1. (a) Schematic plot of the convective tank. Snapshots of vorticity ζ for thermal Rossby number RoT = 5.41 (b) and RoT = 0.03 (c). On the scale bar, Lid = 2.4 cm and Liid = 22.6 cm are the Rossby radius of deformation for (c) and (b), respectively. (d) Kinetic energy spectra, E(k), for various values of RoT. The arrow indicates the wave number kp corresponding to the peak of E(k) when RoT = 0.03. Inset: radial profiles of temporal- and zonal-averaged azimuthal velocity, Uθ. (e) Kinetic energy spectra compensated by k−3 and normalised by N2 versus LRk. The dashed line indicates the plateau segment for LRk ∈ [2, 10] and has a magnitude of ∼ 0.5. Data are for height h = 0.18 m.

 

How to cite: Read, P., Ding, S., Bobas, H., Scolan, H., and Young, R.: A Stratification-Dependent, Enstrophy-Controlled Regime in Baroclinic Turbulence Experiments in the Laboratory, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18700, https://doi.org/10.5194/egusphere-egu26-18700, 2026.

EGU26-19406 | ECS | Posters on site | NP6.4

Emergence of Robust Zonal Jets in a Differentially Heated Rotating Annulus 

Shanshan Ding and Peter Read

The midlatitude atmospheres of gas giant planets are characteristic of strong and persistent zonal jets; however, the processes governing their formation and the associated energy pathways remain less understood. To investigate these mechanisms, we conducted a laboratory study of zonal jets driven by thermal forcing in an annular cylindrical tank partially filled with distilled water as the working fluid. Heating is applied at the outer boundary, cooling at the inner boundary, the bottom is thermally insulated, and the top is a free surface. An array of laser diodes embedded in the inner cylinder generates an annular laser sheet, enabling the measurement of velocity fields at a fixed height using particle image velocimetry. By systematically varying the rotation rate and the imposed temperature contrast, we adjusted the steepness of the free surface, thus the topographic β effect, and the thermal forcing strength, respectively. The non-dimensional controlling parameter, thermal Rossby number, RoT, ranges from 0.0012 to 0.01 and Taylor number, Ta, from 2.3 × 1010 to1.7 × 1011. We discerned the emergence of robust zonal jets, of which the zonal-mean kinetic energy accounts for up to 70% of the total kinetic energy, corresponding to a zonostrophic index of 2.7. In this regime, two coherent and persistent prograde jets form near the inner and outer boundaries. The radial profile of the potential vorticity develops toward a pronounced staircase-like structure, consistent with previous numerical studies (Scott and Dritschel, J. Fluid Mech., 2012). Analysis of the inter-scale energy transfer reveals a dominant interaction between the zonal-mean flow and eddies, while the kinetic energy spectrum of the zonal-mean component exhibits k−5 (where k denotes the wavenumber), in agreement with the theory of zonostrophic turbulence (Sukoriansky and Galperin, PRL, 2002).  

                                 

 Figure 1: A snapshot of azimuthal velocity contour for RoT = 7.1 × 10−3, Ta = 1.44 × 1011 and β =49.7 m−1 s−1.

 

How to cite: Ding, S. and Read, P.: Emergence of Robust Zonal Jets in a Differentially Heated Rotating Annulus, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19406, https://doi.org/10.5194/egusphere-egu26-19406, 2026.

We investigate a laboratory analogue of the Atlantic thermohaline circulation, which is driven by horizontal gradients of thermal and haline forcing at the water surface. The system can exhibit different stable configurations, with a thermally driven overturning flow and a weakened or reversed flow with enhanced stratification driven by the salinity gradient.

A regime transition from the thermally driven to the weak state serves as analogue of a potential future collapse of the Atlantic meridional overturning circulation, and is likely also related to climate changes in paleoclimate history. By change of the surface salinity forcing (emulating increases in polar meltwater input) the system is moved towards and beyond the transition, and changes in the velocity field and tracers are monitored.

It is analyzed whether prior to the stability loss there are statistical early-warning signals in the variability of the turbulent up- and downwelling plumes, and it is determined what are the best observables to detect these. This helps shed light on whether such a regime transition can be viewed as a tipping point in the sense of a saddle-node bifurcation preceded by critical slowing down.

How to cite: Lohmann, J.: Exploring stability, variability, and regime transitions in a laboratory analogue of the ocean's thermohaline circulation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20418, https://doi.org/10.5194/egusphere-egu26-20418, 2026.

EGU26-21329 | ECS | Posters on site | NP6.4

Fast Gravity Waves and Slow Manifolds 

Manita Chouksey and Amjad Hasan Peringampurath

High-frequency internal gravity waves are ubiquitous features in rotating stratified flows, and interact nonlinearly with balanced vortices as well as other waves, resulting in energy transfers across multiple scales. Understanding these multiscale exchanges rests on a precise disentangling of internal waves from the balanced flow in a fully nonlinear flow system. This is the focus of this work, which facilitates the understanding of complex nonlinear mechanisms of internal gravity wave generation, such as spontaneous loss of balance, associated with the notion of the 'slow manifold'.

Here I discuss the generation of internal waves by nonlinear processes: spontaneous emission, symmetric instability, and stimulated emission; through different nonlinear flow decomposition methods: nonlinear normal-mode initialization and nonlinear decomposition at higher orders with asymptotic expansion in Rossby number. Wave generation diagnosed with a different approach, namely optimal balance with and without time-averaging is also compared and discussed. An important result is that wave generation by spontaneous emission is generally weak to negligible, becoming significant only at higher orders and high Rossby numbers. Symmetric instability is more effective in wave generation, also at moderate Rossby numbers. Stimulated emission represents a more realistic scenario of wave emission that might be at play in the real ocean conditions, and is expected to be effective even at low Rossby numbers. The results present a new perspective on internal wave energetics in geophysical flows, and call for reevaluation of the energy transfers in and out of the internal gravity wave compartment. 

How to cite: Chouksey, M. and Peringampurath, A. H.: Fast Gravity Waves and Slow Manifolds, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21329, https://doi.org/10.5194/egusphere-egu26-21329, 2026.

EGU26-21559 | ECS | Orals | NP6.4

Boundaries behaviour of gravity currents 

Antonio Ammendola, Michele Rebesco, Stefano Salon, Federico Falcini, and Federico Roman

Gravity currents are buoyancy-driven flows generated by horizontal density gradients and govern the transport of mass, momentum, and scalars in both natural and engineered systems. A detailed understanding of their near-wall behavior is essential for accurately describing the turbulent mechanisms developing in this region, which is characterized by strong spatial variability, particularly at increasing Reynolds numbers (Re=UbH/ν, with H the initial height of the dense fluid, ν the cinematic viscosity, Ub=(g’H)0.5 a velocity scale related to the reduced gravity g’=g(ρ1- ρ0)/ ρ0, where g is the gravitational acceleration,  ρ1 the density of the heavier fluid and ρ0 the ambient density).  

 Several numerical simulations were performed in straight channels under a lock-exchange configuration using a wall-resolved Large Eddy Simulation. The analyzed cases differ in terms of Reynolds number (in the range 34000-136000), both by increasing the height of the domain and by modifying the density difference. 

The analysis of the near-wall behavior focused on the head of the current, identified through mean density values. Subsequently, streamwise velocity profiles in the wall-normal direction were extracted, first averaged in the spanwise direction and then also along the streamwise direction. Although the latter direction is not homogeneous, this procedure provides an overall view of the behavior of the current head during its temporal evolution. 

The gradient of the streamwise velocity in the wall-normal direction was used to define the boundary-layer thickness δ. It was observed that the temporal evolution of the normalized thickness δ* = δ/H is similar for all the cases analyzed; moreover, after an initial increase, it tends to approach an asymptotic value during the self-similar phase. In accordance with the characteristics of this phase, it is also observed that the mean velocity profile tends to remain invariant over time during the evolution of the current. Moreover, the presence of a logarithmic region is identified, of the form u+=a(lny+)+bu+=aln⁡y++b (where u+=u/u𝜏, and y+=yu𝜏/νy+=yu𝜏/𝜈u𝜏 denoting the friction velocity), with an increase in the slope A (in a logarithmic plot) relative to the canonical value (A=2.44), consistent with the local presence of stable stratification. 

The results obtained may have important implications for the parameterization of simplified large-scale circulation models, particularly with regard to the definition of appropriate boundary conditions. 

How to cite: Ammendola, A., Rebesco, M., Salon, S., Falcini, F., and Roman, F.: Boundaries behaviour of gravity currents, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21559, https://doi.org/10.5194/egusphere-egu26-21559, 2026.

Numerical simulations are performed to investigate the propagation, flow structure, and runout of turbidity currents in regimes where buoyancy-driven dynamics interact with finite settling effects. A Lagrangian particle-tracking framework is used to represent the evolving density field and its coupling with the carrier flow, enabling detailed analysis of current dynamics across multiple flow regimes. 

We first examine the temporal evolution of turbidity currents, which exhibit distinct slumping, propagation, and dissipation stages. The role of finite settling is shown to modulate density stratification and, in turn, the efficiency of momentum transfer within the current. We then analyse flow structure and deposition-induced feedbacks on the current dynamics. Transverse variations in the flow and deposition pattern are associated with lobe-and-cleft structures, while longitudinal variations arise from vortex detachment and decay. Finally, we propose a new scaling law for turbidity-current propagation speed and runout length that incorporates the combined effects of buoyancy forcing and settling-induced density evolution. The numerical results show close agreement with the proposed scaling, supporting its applicability to a wide class of particle-laden density currents. These results provide new insight into the dynamics of turbidity currents as geophysical density currents and contribute to improved predictive frameworks for buoyancy-driven flows in natural environments.

How to cite: Chou, Y.-J. and Yeh, Y.-C.: Propagation and flow structure of turbidity currents in settling regimes: A Lagrangian particle-tracking study, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21650, https://doi.org/10.5194/egusphere-egu26-21650, 2026.

Turbulence in the stably stratified boundary layer is generated by shear, while its development is inhibited by buoyant forces. Due to this interplay, flow regimes with different physical and dynamical characteristics exist. Fully turbulent stable boundary layers, also coined as weakly stable boundary layers, are rather well described by turbulence theory, but the very stable boundary layer is home to unsteady and intermittent turbulence that is less well understood. At high stability in the atmospheric boundary layer, non-turbulent processes on sub-mesoscales (such as dirty waves, drainage flows, etc) become more important, and the flow becomes highly non-stationary. Multiscale data analyses based on different field measurement campaigns show signs of direct energy transfers between sub-mesoscales and turbulent scales, with impacts on the turbulence characteristics. On the one hand, the scale interactions are linked to anisotropic turbulence; on the other hand, turbulence intermittency becomes important when the energy content of the sub-mesoscales becomes an important percentage of the mean kinetic energy.

How to cite: Vercauteren, N., Gucci, F., and Kuttikulangara, A.: Scale interactions in the stably stratified atmospheric boundary layer and impacts on the anisotropy and intermittency of turbulence, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22015, https://doi.org/10.5194/egusphere-egu26-22015, 2026.

EGU26-22097 | ECS | Posters on site | NP6.4

Anisotropic turbulence in the Ekman boundary Layer 

Federica Gucci, Nikki Vercauteren, and Abhishek Paraswarar Harikrishnan

The Ekman boundary layer is driven by the triadic balance of pressure gradient, Coriolis, and friction force. Under strongly stable stratification, the flow can become globally intermittent, with large-scale motions controlling the spatial organisation of quasi-laminar patches of fluid that extend from the outer layer down to the surface layer. Stable stratification additionally affects the Ekman spiral, making it shallower and characterized by a faster veering of the wind vector compared to neutral stratification, resulting in stronger directional wind shear.

In the present contribution, a dataset from direct numerical simulations (DNS) of a turbulent Ekman flow over a smooth and flat wall is used to investigate how the spatial organization of a globally intermittent flow and the modified Ekman spiral shape the anisotropy of the stress tensor. Multiple studies have shown that small-scale turbulence becomes more anisotropic with increasing stratification, with frequent occurrence of one-component anisotropic stress tensors (i.e. kinetic energy distributed along one dominant direction) that also characterizes the large scales. Previous analyses of small-scale coherent vortical structures in these DNS revealed that hairpin vortices within a turbulent patch of a globally intermittent flow are aligned along the same direction, which may contribute to shaping the anisotropy of the stress tensor at the large and small scales.

Scale-wise analyses of the flow and its stress anisotropy under strongly stable stratification and neutral stratification are performed to investigate these features. Results show that large-scale motions found in the outer layer are associated with a dominant energy-containing length scale that extends down to the inner layer. As a result, the energy spectrum in the inner layer has two dominant length scales, with shear-driven turbulence associated with the smaller length scale. Directional wind shear contributes to large-scale anisotropy as the surface is approached. Due to the strong coupling arising from global intermittency, information on anisotropy is transferred from the outer layer down to the surface layer.

How to cite: Gucci, F., Vercauteren, N., and Harikrishnan, A. P.: Anisotropic turbulence in the Ekman boundary Layer, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22097, https://doi.org/10.5194/egusphere-egu26-22097, 2026.

Traditional operational weather prediction systems are driven by physics-based numerical simulations, which demand substantial computational resources. With the advancement of Artificial Intelligence (AI), modern transformer architectures have emerged as powerful alternatives, delivering high accuracy in data-driven weather forecasting. Despite this progress, transformers inherently operate on discrete representations and do not follow the underlying physical laws, thereby limiting their effectiveness in modelling the continuous spatio-temporal evolution of atmospheric processes. To mitigate this issue and inject physical structure, we introduce continuous-depth dynamics within the encoder and attention mechanism of a transformer. We propose the dual attention mechanism that jointly captures spatial and temporal dependencies. The spatial mode is modelled as a simple multi-head attention which is fused with the temporal component. The temporal attention operates on finite-difference derivatives of token embeddings across successive time steps, allowing the network to infer local temporal gradients and represent continuous evolution in feature space. Furthermore, we introduce continuous-depth Neural ODE layers in transformer encoder which models smooth transitions replacing the discrete residual updates. Finally, we propose a customized physics-informed loss function which is applied during training as a soft-constraint. This loss penalizes deviations from established thermodynamic and kinetic energy relationships governing temperature and wind evolution. By constraining the learned dynamics to respect these physical laws, the model produces forecasts that are not only data-accurate but also energetically consistent with the underlying principles of the atmospheric system.

How to cite: Saleem, H., Salim, F., and Purcell, C.: PINN-Cast: Exploring the Role of Continuous-Depth NODE in Transformers and Physics Informed Loss as Soft Physical Constraints in Weather Forecasting, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-78, https://doi.org/10.5194/egusphere-egu26-78, 2026.

EGU26-526 | ECS | Posters on site | AS1.2

Hima-Net: Deep Learning Enhancement of ECMWF S2S Winter Precipitation Forecasts over Northern India 

Junaid Dar and Subimal Ghosh

Seasonal climate forecasts are critical for disaster management across the fragile Himalayan ecosystem, particularly during winter. However, these forecasts often exhibit strong spatial and temporal biases that reduce their reliability for predicting extremes at longer lead times. Traditional postprocessing methods such as quantile mapping and linear scaling assume stationarity and have limited ability to capture complex spatiotemporal error structures. To address these limitations, this study introduces Hima-Net (Himalayan-Net), a hybrid deep learning model that combines U-Net and Conv-LSTM architectures. Hima-Net is designed to improve the skill of sub-seasonal-to-seasonal (S2S) daily precipitation forecasts from the ECMWF S2S system by learning season-specific spatial and temporal patterns in forecast errors. The model is trained with a loss function that jointly emphasizes magnitude and correlation, enhancing its ability to represent the distribution and evolution of precipitation across lead times. Evaluation using metrics such as root mean square error (RMSE) and anomaly correlation coefficient (ACC) shows that Hima-Net consistently outperforms the raw forecasts across lead times over the Himalayan region. These findings demonstrate the potential of deep learning–based postprocessing to better capture and enhance spatial and temporal forecast patterns, offering a promising pathway for more accurate wintertime precipitation forecasts over the complex terrain of the Himalayas.

How to cite: Dar, J. and Ghosh, S.: Hima-Net: Deep Learning Enhancement of ECMWF S2S Winter Precipitation Forecasts over Northern India, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-526, https://doi.org/10.5194/egusphere-egu26-526, 2026.

Global Navigation Satellite System Radio Occultation (GNSS RO) observations are increasingly important for improving atmospheric profiling and numerical weather prediction (NWP), especially in cloudy, moisture-rich tropical environments where other satellite observations are often degraded. This study presents two complementary advances: (1) an improved regional quality-control strategy for preserving COSMIC-2 bending-angle data in cloudy regions, and (2) an assessment of the impact of assimilating Tianmu-1 RO observations from a newly deployed 23-satellite commercial constellation on the prediction of Typhoon Gaemi (2024).

First, we show that the widely used latitude-based quality control of COSMIC-2 bending-angle data leads to excessive removal of observations between 6–8 km near the Solomon Islands, where persistent summertime altostratus frequently reach above 6 km. Despite the long-wavelength nature of RO measurements—which makes them less sensitive to clouds—these regions were incorrectly flagged as outliers. By implementing a 2.5° × 2.5° local quality-control approach, the number of discarded observations in cloudy areas is substantially reduced, yielding a more spatially uniform deviation structure relative to the local mean. This regionally adaptive method better preserves high-quality RO data in both mid-tropospheric altostratus and lower-tropospheric Intertropical Convergence Zone environments.

Second, we evaluate the impact of assimilating over 30,000 daily RO profiles from the Tianmu-1 constellation using the GSI–WRF system. Assimilating Tianmu-1 data alone—without other satellite observations—reduces 120-hour track errors of Typhoon Gaemi by 20–40%, with the largest improvements beyond 48 hours. Diagnostics show that enhanced prediction skill arises mainly from improved inner-core temperature structure and better representation of the large-scale steering flow. Remarkably, the track forecasts with Tianmu-1 assimilation are even slightly better than the operational forecasts from the NCEP Global Forecast System (GFS).

Overall, these results highlight the increasing importance of high-density GNSS RO constellations in forecasting tropical cyclone intensity and track, and emphasize the value of cloud-aware, adaptive regional quality-control techniques in preserving cloud-affected observations. Future work will extend these adaptive quality-control strategies globally and examine synergistic assimilation of COSMIC-2, Tianmu-1, and other commercial RO datasets.

How to cite: Yang, S. and Zou, X.: Positive Impacts of Tianmu-1 RO Data Assimilation on Tropical Cyclone Forecasts and the Non-negligible Influence of Altostratus Clouds on RO Data Quality, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1396, https://doi.org/10.5194/egusphere-egu26-1396, 2026.

Satellite brightness temperature (BT) observations contain rich information about the horizontal distributions of cloud and rainfall structures; while radiosonde observations provide high-vertical-resolution measurements of temperature, moisture, and wind in the atmosphere. Beyond their traditional use in assimilation and retrieval, this study demonstrates innovative quantitative uses of BT and radiosonde observations for evaluating high-resolution numerical weather prediction (NWP) simulations of tropical cyclones (TCs) and Southwest Vortices (SWVs).

First, we apply BT observations to document  the structural evolution of TCs and SWVs and to directly compare simulated hydrometeor distributions with satellite-observed cloud and precipitation features. These BT-based diagnostics provide objective constraints on model representation of convective initiation and development as well as the impact of diurnal variability.

Second, a BT-based threat-score (BT-TS) framework is introduced to assess the skill of rainfall forecasts with respect to satellite BT observations instead of rainfall observations traditionally used in TS evaluation. Using microwave humidity-sounder channels, the BT-TS metric performs well for assessing rainfall forecast in regions where precipitation observations are sparse or unavailable. The BT-TS forecast results highlight model deficiencies in timing, extent, and intensity of SWV-induced convective rainfall.

Third, radiosonde profiles are used to investigate lower-tropospheric processes critical for vortex evolution, focusing on planetary boundary layer (PBL) height and vertical variability under different vertical-resolution configurations. Verification with high-vertical-resolution (~5–6 m) profiles from 119 Chinese radiosonde stations during the summers of 2021–23 shows that accurately representing PBL height and lower-tropospheric thermodynamic variability requires approximately doubling  the number of ERA5 vertical levels.

Together, these BT- and radiosonde-based diagnostics provide a comprehensive observational framework for evaluating the structural evolution of TCs and mesoscale SWVs. Future work will leverage these insights to refine cloud microphysics schemes, optimize model vertical-resolution design, and enhance the predictability of convection-permitting NWP systems.

How to cite: Zou, X.: Besides Assimilation and Retrieval: Innovative Quantitative Uses of Satellite Brightness Temperatures and Radiosonde Observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1397, https://doi.org/10.5194/egusphere-egu26-1397, 2026.

EGU26-2677 | ECS | Posters on site | AS1.2

Bias-correction of wind speeds to improve PM2.5 predictability in chemical transport model 

Jaehee Kim, Jinhyeok Yu, Hyun S. Kim, Soon-young Park, Jung-Hun Woo, and Chul H. Song

Wind speed is a critical factor influencing the transport and dispersion of atmospheric pollutants in air quality models. However, numerical weather prediction (NWP) models, such as the weather research and forecasting (WRF) model, typically overestimate surface wind speeds, leading to inaccuracies in air quality predictions. To address this limitation, we developed an Artificial Intelligence (AI)-based Wind Field Correction (WFC) model aimed at improving PM2.5 forecasts over East Asia. The WFC model was constructed using the eXtreme Gradient Boosting (XGBoost) algorithm and trained on eight years of data, incorporating WRF-simulated meteorological variables as input features and in situ, ship-based, buoy, and radiosonde observations as targets. The WFC model effectively reduced the positive bias in WRF-simulated wind speeds, achieving a 90.15% reduction at the surface level and a 94.6% reduction from the surface to 850 hPa. The bias-corrected wind fields, when incorporated into the GIST Multiscale Air Quality model (GMAQ v1.0) developed by the Gwangju Institute of Science and Technology (GIST), resulted in substantial improvements in PM2.5 predictablity. In Central Eastern China (CEC), the wind field correction mitigated the underestimation of PM2.5 by suppressing excessive plume dilution in the model. In South Korea (SK), the correction slowed down accelerated plume advection, leading to a closer agreement between the simulated and observed PM­2.5 plume locations. In addition, the correction enhanced the representation of daily PM­2.5 variability and improved statistical metrics over the capital cities of Seoul and Beijing.

How to cite: Kim, J., Yu, J., Kim, H. S., Park, S., Woo, J.-H., and Song, C. H.: Bias-correction of wind speeds to improve PM2.5 predictability in chemical transport model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2677, https://doi.org/10.5194/egusphere-egu26-2677, 2026.

Minimizing pixel-wise errors in precipitation nowcasting inherently biases models toward smooth predictions, causing failures in resolving extreme convective events. To address this, we propose IMPA-Net, a meteorology-aware framework centered on spectral consistency. The architecture integrates three innovations: a parameter-free Spatial Mixer to encode multi-variate physical interactions (e.g., terrain-wind coupling); an Integrated Multi-scale Predictive Attention (IMPA) module to capture dynamics from Meso-β to Meso-γ scales; and a Meteorology-Aware Dynamic Loss (MAD-Loss) that employs asymmetric penalties to counteract regression-to-the-mean. Experiments demonstrate a 37.3% relative improvement in HSS for severe convection (45 dBZ). Crucially, RAPSD analysis confirms that IMPA-Net maintains spectral energy consistency across high-frequency bands, enabling it to successfully simulate the complex "dissipation-initiation" lifecycle that existing baselines fail to capture. These findings validate that integrating domain knowledge advances the physical plausibility of data-driven forecasting.

How to cite: He, G. and Cui, H.: IMPA-Net: Meteorology-Aware Multi-Scale Fusion and Dynamic Loss for Extreme Radar-Based Precipitation Nowcasting, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3224, https://doi.org/10.5194/egusphere-egu26-3224, 2026.

EGU26-8109 | ECS | Posters on site | AS1.2

Deep Learning-Based Precipitation Nowcasting for Operational and Flash-Flood Applications 

Rodrigo Almeida, Jamil Göttlich, Noelia Otero, Marian Jurasek, Ladislav Méri, Zinaw Dingetu Shenga, Aitor Atencia, and Jackie Ma

Accurate short-term precipitation nowcasting is crucial for disaster risk reduction, flash-flood early warning, and water resource management. Conventional nowcasting approaches, such as extrapolation-based radar methods or numerical weather prediction models, often struggle to capture the nonlinear evolution of convective systems and are computationally demanding for rapid updates at high spatial and temporal resolution. The ability to provide reliable high-resolution forecasts at lead times of minutes to hours is particularly important for mitigating the societal and economic impacts of intense rainfall events. Recent developments in deep learning (DL), in combination with high-resolution radar observations, represent a compelling alternative for improving short-term precipitation forecasting. Radar-based precipitation data are particularly well suited for nowcasting applications due to their fine spatio-temporal resolution and ability to capture the dynamic structure and movement of precipitation systems. In this study, we develop and evaluate an operationally oriented DL framework for precipitation nowcasting that integrates multi-source data including high-resolution radar and satellite observations and automatic weather station measurements via the qPrec system over Slovakia. By incorporating satellite-derived forcing, the framework accounts for convection initiation and cloud development stage, providing a physical advantage over both classical extrapolation and radar-only deep learning methods. The framework leverages modern DL architectures, including convolutional encoder-decoder models such as U-Net and spatio-temporal transformer-based models (e.g., Earthformer), to learn the temporal evolution of precipitation fields inputs. The use of transformer-based models allows the network to capture long-range spatial dependencies and complex motion patterns that traditional CNNs may miss.

The proposed models generate precipitation forecasts at a spatial resolution of 1 km and a temporal resolution of 5 minutes, with lead times of up to 60 minutes. In addition to instantaneous precipitation estimates, the framework produces 15-minute accumulated precipitation for horizons up to 120 minutes. Unlike traditional methods where predictability skill remains static across resolutions, our DL approach leverages varied spatial representations to enhance predictability at these coarser temporal scales, optimizing the forecast for different hydrological requirements. These accumulated fields can be directly applied to flash-flood hazard assessment, enabling estimation of flood likelihood as a function of rainfall intensity and duration. Model performance is evaluated using standard verification metrics such as the Fractions Skill Score, and continuous ranked probability score (reducing to MAE on deterministic outputs), showing improvement over conventional radar extrapolation methods. This study demonstrates that modern DL approaches, particularly when combined with high-resolution radar observations, offer a promising path toward next-generation operational nowcasting.

How to cite: Almeida, R., Göttlich, J., Otero, N., Jurasek, M., Méri, L., Shenga, Z. D., Atencia, A., and Ma, J.: Deep Learning-Based Precipitation Nowcasting for Operational and Flash-Flood Applications, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8109, https://doi.org/10.5194/egusphere-egu26-8109, 2026.

EGU26-9075 | ECS | Orals | AS1.2

SR-Weather: Super-Resolution Machine Learning Weather Forecast for 1-km Air Temperature Prediction 

Hyebin Park, Seonyoung Park, Daehyun Kang, and Jeong-Hwan Kim

Machine learning-based global weather forecasts often suffer from coarse spatial resolution, limiting their ability to capture fine-scale temperature variability in regions with complex terrain or strong urban–rural gradients. We present SR-Weather, a two-stage deep learning framework that downscales coarse 0.25° forecasts into 1 km air temperature fields. Our model is trained using ERA5 and MODIS-derived temperature data, and leverages high-resolution auxiliary inputs, including elevation, impervious surface fraction, and spatial information–normalized air temperature to enhance spatial fidelity. Applied to 7-day lead forecasts from the FuXi model, SR-Weather consistently outperforms FuXi’s own 1-day lead predictions, indicating strong capabilities in both resolution enhancement and bias correction. The model also exhibits robustness under cloud-contaminated MODIS observations by reconstructing missing temperature values using auxiliary data. While developed and validated over South Korea, SR-Weather is region-agnostic and applicable globally due to the availability of MODIS inputs and minimal reliance on localized data. These results position SR-Weather as a scalable solution for high-resolution, ML-based weather forecasting.

How to cite: Park, H., Park, S., Kang, D., and Kim, J.-H.: SR-Weather: Super-Resolution Machine Learning Weather Forecast for 1-km Air Temperature Prediction, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9075, https://doi.org/10.5194/egusphere-egu26-9075, 2026.

EGU26-10225 | ECS | Orals | AS1.2

Bridging AI Large Meteorological Models and Solar Irradiance Forecasting Through Machine Learning Approaches 

Mingyu Yan, Ming Zhang, Kun Yang, Zhifeng Shu, and Changkun Shao

Renewable energy sources have an increasingly pivotal role in global electricity generation, which poses challenges to the accurate and efficient meteorological forecasting (such as solar irradiance and hub-height wind speed). The development of AI large models has significantly shortened the time required for medium-range global weather forecast. However, their outputs typically lack high-temporal-resolution solar irradiance (e.g., provided only at 6-hour intervals or not at all), which cannot be directly applied to renewable energy forecasting.

In this work, we propose a machine learning framework to integrate the output variables from AI large models with high-resolution solar irradiance forecasting. Specifically, we train XGBoost models at 15 sites in eastern China using ERA5 reanalysis variables (2020–2023) as inputs and hourly surface solar irradiance derived from Himawari-8/9 satellite as targets. The trained models are evaluated on a 2024 test set driven by ERA5, achieving an annual mean hourly RMSE of 88.5 W m-2.

To assess the performance of this approach in medium range forecasting, we use hourly forecasts from the GDAS-driven Pangu Weather Model during January and July 2024 as inputs. Over 20 medium-range forecast tests, our approach (Pangu-ML) yields a day-ahead (24-h lead) RMSE of 62.5 (January) /95.4 (July) W m-2 and a 10-day lead RMSE of 92.3 (January) /110.1 (July) W m-2. For comparison, we conduct parallel simulations using the GFS-driven WRF v4.6 model at 9-km resolution over eastern China. The WRF-based irradiance forecasts produce day-ahead and 10-day RMSEs of 78.4 (January) /107.6 (July) W m-2 and 109.8 (January) /130.3 (July) W m-2 across the 15 sites, demonstrating that Pangu-ML achieves comparable or even superior accuracy.

In summary, our approach takes advantage of the computational efficiency of AI large meteorological models. It enables rapid generation of solar irradiance forecasts with minimal computational cost, thereby offering a practical pathway for subsequent operational ensemble irradiance forecasting.

How to cite: Yan, M., Zhang, M., Yang, K., Shu, Z., and Shao, C.: Bridging AI Large Meteorological Models and Solar Irradiance Forecasting Through Machine Learning Approaches, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10225, https://doi.org/10.5194/egusphere-egu26-10225, 2026.

EGU26-10396 | ECS | Posters on site | AS1.2

Ensemble Experiments in an AI-NWP Coupled Framework: A Typhoon Case 

Yangjinxi Ge

Artificial intelligence (AI) models have demonstrated advancements in computational efficiency and forecast accuracy relative to the Numerical Weather Prediction (NWP), but they are unable to fully represent high-dimensional atmospheric dynamics. Thus, some AI-NWP coupled frameworks have been proposed, such as integrating AI-driven boundary conditions with numerical models to leverage the strengths of both approaches. However, in this coupled framework, ensemble forecasts and associated error propagation and energy dynamics remain under-explored. In this study, an AI-NWP coupled system that also uses the stochastic kinetic energy backscatter scheme (SKEBS) to generate ensemble forecasts is established. Ensemble simulations of Typhoon Yutu (2018) are carried out with the Weather Research and Forecasting (WRF) model employing Pangu-Weather and FuXi forecast data as boundary forcing. The results show that the ensemble WRF_Pangu (WRF_FuXi) improved Yutu’s track forecast by 67% (50%) compared to the traditional physics-based WRF_GFS (Global Forecast System), and reduced its intensity underestimation by about 67% relative to their AI global counterparts. Nonetheless, WRF_FuXi and WRF_Pangu exhibited limited ensemble spread and linear error growth, reflecting deterministic tendencies. Comparison of global and regional experiments show that Pangu-Weather is more physically constrained and thus better aligned with the WRF model for regional applications, while the adaptation of FuXi to the regional model is less robust. Spectral analysis revealed that AI-derived boundaries introduced excessive small-scale energy and underestimated larger-scale energy. The regional model WRF acted as a “conveyor belt”, propagating additive small-scale energy upscale, ultimately overwhelming the stochastic perturbations for ensemble generation. These findings underscore the need to incorporate more physical features into the AI-derived boundary conditions for ensemble forecasting.

How to cite: Ge, Y.: Ensemble Experiments in an AI-NWP Coupled Framework: A Typhoon Case, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10396, https://doi.org/10.5194/egusphere-egu26-10396, 2026.

EGU26-11158 | ECS | Orals | AS1.2

ML-based time interpolation of AIFS Ensemble for renewable energy forecasting 

Hans Brenna Schjønberg, Riccardo Parviero, Marius Koch, and Alberto Carpentieri

Recent advancements in machine learning based weather prediction (MLWP) present novel opportunities for downstream applications like forecasting of renewable energy production from intermittent sources, like wind and solar. MLWP models guarantee shorter simulation run times and lower computational costs, allowing faster updates of downstream models and greater flexibility in the generation of weather scenarios.

Forecasting renewable energy generation critically depends on available weather forecast data at adequate temporal and spatial resolution. Using MLWP weather data in energy system modelling and forecasting has been limited by the coarse temporal resolution of the current generation of models (e.g. ECMWF’s AIFS Ensemble model runs at 6-hour time steps).

In Europe, power market participants are increasingly exposed to weather forecast inaccuracies. This is due to the combined effect of how the power price is calculated for each price area, and the recent increase in intermittent renewable installed capacities. In detail, power prices are set each day for the following day by balancing supply and demand for each Market Time Unit (MTU), which are now 15 minutes long. It is then massively important to benchmark weather forecasts on a time resolution closer to the power market MTU, to properly assess which period will potentially be oversupplied, or undersupplied from intermittent renewable sources. In this context, the 6-hour time resolution of current MLWP models becomes a significant limiting factor for their usefulness.

Using NVIDIA’s Earth2Studio framework, we demonstrate an efficient, integrated MLWP pipeline combining the [open source] AIFS model with the ModAFNO time interpolation model to provide 1-hourly time-resolution MLWP data. This interpolated data is applied to our intermittent renewable energy production models to assess the interpolation quality compared the uninterpolated AIFS data and the best-in-class numerical weather prediction data provided by ECMWF’s IFS Ensemble forecast.

How to cite: Brenna Schjønberg, H., Parviero, R., Koch, M., and Carpentieri, A.: ML-based time interpolation of AIFS Ensemble for renewable energy forecasting, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11158, https://doi.org/10.5194/egusphere-egu26-11158, 2026.

EGU26-11583 | ECS | Posters on site | AS1.2

Impacts of subgrid-scale orographic drag on landfalling typhoon precipitation 

Ming Zhang, Mingyu Yan, Yulong Ma, Kun Yang, and Zhifeng Shu

While the effects of subgrid orographic drag on large-scale circulation have been extensively studied, its influence on typhoon precipitation remains less understood. Using the Weather and Research Forecasting model, this study investigates impacts of subgrid orographic drag components (gravity wave drag (GWD), flow-blocking drag (FBD), and turbulent orographic form drag (TOFD)) on landfalling typhoon precipitation and explores their resolution sensitivity through two representative cases: Super Typhoon Lekima (2019) and Severe Typhoon In-Fa (2021). Results reveal distinct distributions of GWD and TOFD over southeastern coastal China, which significantly modulate precipitation during strong landfalls like Lekima: GWD enhances precipitation in southern land areas affected by the typhoon while suppressing it in northern regions, whereas TOFD exerts precisely opposing effects. This is mainly due to enhanced (weakened) lower-tropospheric wind speed and water vapor transport caused by GWD (TOFD). GWD is highly sensitive to horizontal resolution, exhibiting more pronounced effects on the wind, moisture, and precipitation at coarser resolutions, while TOFD remains relatively invariant to horizontal resolution changes. Resolution of subgrid orography dataset driving these parameterizations is essential for accurately simulating drag distributions and impacts. Finally, typhoon intensity modulates these effects: stronger background circulation exacerbates the precipitation impacts of both GWD and TOFD.

How to cite: Zhang, M., Yan, M., Ma, Y., Yang, K., and Shu, Z.: Impacts of subgrid-scale orographic drag on landfalling typhoon precipitation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11583, https://doi.org/10.5194/egusphere-egu26-11583, 2026.

Extreme precipitation poses significant risks to society and infrastructure, highlighting the urgent need for accurate short-term nowcasting. While deep learning models have shown promise in precipitation forecasting, they often lack integration with physical principles, leading to inconsistencies and limited skill in predicting convective evolution. In this study, we introduce RainCast—a novel generative nowcasting framework that synergistically combines deterministic physical modeling with stochastic generative networks to improve the accuracy and physical consistency of extreme rainfall forecasts.

RainCast integrates a deterministic branch based on Neural Ordinary Differential Equations (Neural ODE) to simulate large-scale advective processes and a generative branch built upon a conditional diffusion model to capture fine-scale stochastic variability. The model is guided by key physical features such as flow fields, vorticity, and divergence derived from dual-polarization radar observations, which provide essential dynamical information about convective systems. We train and evaluate the framework using vertically integrated liquid water (VIL) data from dual-polarization radars in China (GD-SPOL) and North America (SEVIR).

Quantitative assessments demonstrate that RainCast significantly outperforms existing nowcasting methods such as SimVP, SwinLSTM, and NowcastNet. On the GD-SPOL dataset, RainCast improves the Critical Success Index (CSI) for intense convection (VIL ≥ 160) by up to 14.1% at 90-minute lead times. Structural similarity metrics also show substantial gains, with reductions in Fréchet Video Distance (FVD) by 25.4% and Learned Perceptual Image Patch Similarity (LPIPS) by 44.6%. Case studies further illustrate RainCast’s ability to realistically simulate the evolution of organized convective systems, including squall lines and multicell storms, while maintaining physical coherence in wind field retrievals.

Our results underscore the value of embedding physical guidance into generative deep learning architectures for convective nowcasting. The RainCast framework represents a meaningful step toward more reliable, interpretable, and physically consistent nowcasting of extreme precipitation, with potential applications in operational meteorology and disaster preparedness.

How to cite: Pan, X. and Zhao, K.: Physics-Guided Generative Nowcasting of Extreme Precipitation with Dual-Polarization Radar and Neural ODE-Diffusion Framework, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11714, https://doi.org/10.5194/egusphere-egu26-11714, 2026.

The forecast skill of the Probability Matching Method (PMM) was evaluated based on ensemble precipitation forecasts over New Zealand, with a detailed analysis of the influence of New Zealand's topography. This study used New Zealand ensemble forecast data in 2023 and employed multiple objective verification methods to statistically analyze the difference in performance of PMM over mountainous and plain areas of New Zealand. Results indicate that topographic factors cause significant differences in the skill of the ensemble mean (EM) and PMM between mountainous and plain regions of New Zealand. In the mountainous areas of New Zealand, the performance of the EM is largely comparable to, or slightly better than, PMM. In contrast, PMM outperforms the EM over plain areas. The primary reason for this difference is that the most precipitation affecting New Zealand, moving from west to east, first encounters the western mountainous regions. The unified topography induces uplift motions in all ensemble members, resulting in high spatial consistency in precipitation patterns over the mountains. The smoothing effect caused by inter-member differences is thus weaker. Over plain areas, however, the lack of uniform topographic forcing makes precipitation more sensitive to differences in flow-over-mountain conditions and local thermal-dynamic conditions, leading to greater relative differences among members. Consequently, PMM exhibits higher forecast skill relative to the EM in plains. This also gives PMM a greater advantage over the North Island of New Zealand, as the topographic influence is more dominant in the South Island.

How to cite: Qiao, X. and Cattoën, C.: The Impact of New Zealand's Topography on Quantitative Precipitation Forecasting Based on the Probability Matching Method, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13092, https://doi.org/10.5194/egusphere-egu26-13092, 2026.

EGU26-13981 | ECS | Orals | AS1.2

SALAMA 1D: Deep-learning-based identification of thunderstorm occurrence in NWP forecasts without relying on convective indices 

Kianusch Vahid Yousefnia, Christoph Metzl, and Tobias Bölle

Thunderstorms pose significant risks to society and the economy due to hazards such as heavy precipitation, hail, and strong winds, which is why accurate forecasts are required to mitigate their impacts. Convection-permitting numerical weather prediction (NWP) models can explicitly resolve convective processes, but predicting thunderstorms from their output remains challenging since there is no obvious state variable that directly indicates thunderstorm occurrence. Instead, many approaches rely on combining multiple convective indices, such as convective available potential energy (CAPE), which are derived from state variables like temperature, pressure, and specific humidity, and act as surrogates for thunderstorms.

In this study, we present a deep neural network model that bypasses surrogate variables and instead directly processes the vertical profiles of state variables provided by convection-permitting forecasts. Our model, SALAMA 1D, analyzes ten different NWP output fields, such as wind velocity, temperature, and ice particle mixing ratios, across the vertical dimension, to produce the corresponding probability of thunderstorm occurrence. The model’s architecture is motivated by physics-based considerations and symmetry principles, combining sparse and dense layers to produce well-calibrated, pointwise probabilities of thunderstorm occurrence, while remaining lightweight.

We trained our model on two summers of forecast data from ICON-D2-EPS, a convection-permitting ensemble weather model for Central Europe operationally run by the German Meteorological Service (DWD), using the lightning detection network LINET as the ground truth for thunderstorm occurrences. Our results demonstrate that, up to lead times of (at least) 11 hours, SALAMA 1D outperforms a comparable machine learning model that relies solely on thunderstorm surrogate variables. Additionally, a sensitivity analysis using saliency maps indicates that the patterns learnt by our model are to a considerable extent physically interpretable. Finally, we show that spatial coverage can be extended to all of Europe by retraining on ICON-EU reanalysis data. Our work advances NWP-based thunderstorm forecasting by demonstrating the potential of deep learning to extract predictive information from high-dimensional NWP data—without sacrificing model interpretability.

How to cite: Vahid Yousefnia, K., Metzl, C., and Bölle, T.: SALAMA 1D: Deep-learning-based identification of thunderstorm occurrence in NWP forecasts without relying on convective indices, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13981, https://doi.org/10.5194/egusphere-egu26-13981, 2026.

EGU26-15394 | Posters on site | AS1.2

Linking the Weather Generator with Weather Forecasts for Use in Forecasting Weather-Dependent Processes  

Martin Dubrovsky, Miroslav Trnka, Lenka Bartosova, Petr Stepanek, Eva Pohankova, and Jan Balek

Weather Generator (WGs) are tools, which produce synthetic weather series which are statistically similar to the weather series used to calibrate the WG. Though the underlying models of the WGs (frequently based on Markov chains and autoregressive models) include a prognostic component, so that the WGs could be hypothetically used to make a weather forecast, the precision of such forecast quickly converge (with increasing lead time) to zero. In our contribution, we do not use our generator for weather forecasting, but we use it to produce an ensemble of synthetic weather series which fit an available weather forecast.  

One of the hot challenges in agrometeorology is a seasonal crop yield forecasting, which is a critical aspect of food production planning. The seasonal crop yield forecasting may be based on crop growth models run with daily time step. In this approach, the meteorological data fed into these models typically consist of observational weather data up to the forecast date, followed by weather forecast data (WF), mean climatic data, or weather generators (WGs).

In our contribution, we propose an improvement of the WG-based methodology. In contrast to approaches described in the literature, where WGs synthesize data independently of any WF, we are developing a methodology in which our single-site parametric M&Rfi WG (run with daily step) synthesizes multiple realisations of weather series which fit available WFs. Two approaches are proposed: (A) For use in operational crop yield forecasting, WG produces synthetic weather series starting with D0 day (which comes after the last day with weather observations and for which WF is available), so that the synthetic series smoothly follows available observations. In our experiments, (a) WF is defined for the upcoming days/weeks/months either in terms of the absolute values of individual weather variables or deviations from their climatological normals, (b) WF may optionally include information on its accuracy (e.g. in terms of standard errors or min-max intervals), (c) Precipitation forecast is assumed to be given in terms of amount and probability of precipitation occurrence, (d) WF may be defined separately for a set of time intervals (e.g. for next three days, next week, next months, etc.). The procedure for linking the generation process with WF is based on a continuous adjusting the stochastically generated series in a way resulting in a series that fits the WF while the internal structure (e.g. relations between variables) of the series remains realistic. (B) the “Research” approach: Unlike A approach, the B approach aims to answer the question: How the use of WF of given accuracy may contribute to the accuracy of seasonal forecast of the crop yields? The process of adjusting the stochastically generated series is similar to A method, but now, we care only about the dispersion of individual realisations, so that the magnitude of the dispersion corresponds to the known accuracy of the weather forecast.

Acknowledgements: The experiments were made within the frame of projects PERUN (supported by TACR, no SS0203004000), OP JAK (supported by MSMT, no. CZ.02.01.01/00/22_008/0004605) and AdAgriF (supported by MSMT, no. CZ.02.01.01/00/22_008/0004635).

How to cite: Dubrovsky, M., Trnka, M., Bartosova, L., Stepanek, P., Pohankova, E., and Balek, J.: Linking the Weather Generator with Weather Forecasts for Use in Forecasting Weather-Dependent Processes , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15394, https://doi.org/10.5194/egusphere-egu26-15394, 2026.

EGU26-15508 | Orals | AS1.2

AI nowcasting of localized heavy precipitation from fast-scanning radar with probabilistic and 3D motion guided prediction 

Philippe Baron, Shigenori Otsuka, Adrià Amell, Seiji Kawamura, Shinsuke Satoh, and Tomoo Ushio

Accurate real-time prediction of heavy precipitation is essential for disaster prevention. It remains a challenge for operational meteorology, especially for sudden localized convective storms for which traditional radar and observation extrapolation methods struggle to capture their rapid vertical development, which typically originate at altitudes of 4--8 km before descending to the surface in about 10 minutes.  

In Japan, three Multi-Parameter Phased Array Weather Radars (MP-PAWR) generating 3D data every 30 seconds with high vertical resolution have been deployed. Leveraging these dense 4D observations, an AI-based model produces real-time nowcasts (very short-term forecasts) with high-resolution of 500 m and 10-minute lead time. Updated every 30 seconds, our nowcasts outperform traditional methods for predicting the onset and the dissipation of localized convective precipitation. However, performance is degraded during the mature phase of the storm when its structure becomes more complex (e.g., overlapping  convective cells in different lifecycle states, domination of horizontal motion in radar pattern changes) (Baron et al., 2025a).

Two major improvements are currently being investigated: 1) a Quantile Regression Neural Network (QRNN) technique has been integrated to assess the probability distribution of possible nowcasts and thus provide credible intervals (Baron et al., 2025b), and 2) a better representation of 3D motion is being implemented, as it plays a critical role during the mature phase of storms. The new version of the model will integrate two separate modules: one specialized for capturing 3D-motion vectors, while the second predicts rainfall intensity with motion guidance. Both modules use the current nowcast model architecture which has demonstrated solid performance. The motion module is trained using 3D motion vectors derived directly from the radar observations through a 3D Tracking Radar Echoes by Correlation (TREC) method originally designed for PAWR extrapolation (Otsuka et al., 2016).

This study will present these developments with a special focus on the motion guidance module that is being implemented. The limitations of our approach will also be discussed (e.g., QRNN vs diffusion model, TREC limitation for weak gradient cases, no information on rain precursors and mesoscale scales).

Baron et al., 2025a: “Real-time nowcasting of sudden heavy rainfall using artificial neural network and multi-parameter phased array radar”, SOLA, https://doi.org/10.2151/sola.2025-039

Baron et al., 2025b: “3D Precipitation Nowcasting from Phased Array Radar with Uncertainty Estimation Using a Quantile Regression Neural Network”, IEEE RadarConf25,  10.1109/RadarConf2559087.2025.11204931

Otsuka et al., 2016: Precipitation nowcasting with three-dimensional space–time extrapolation of dense and frequent phased-array weather radar observations. Wea. Forecasting, 31, 329–340.

How to cite: Baron, P., Otsuka, S., Amell, A., Kawamura, S., Satoh, S., and Ushio, T.: AI nowcasting of localized heavy precipitation from fast-scanning radar with probabilistic and 3D motion guided prediction, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15508, https://doi.org/10.5194/egusphere-egu26-15508, 2026.

The development of various AI models in recent years has been very promising; the models’ ability to train from reanalysis datasets and evaluate on various metrics opened the door for a variety of new applications. However, the real stress test of any new model is its operational performance - applying predictions to data that weren't available during the model development and assessing the model’s capabilities for predicting real-world scenarios previously unseen. 

In August 2025, we deployed our first high-resolution AI-based model for Iceland and it has been providing us with continuous predictions since then. Here we evaluate forecast skill against surface observations and benchmark against NWP models from the United Weather Centres (UWC) in Denmark and Iceland and our local operational NWP model for Iceland. We analyze the model’s strengths and weaknesses in predicting various weather events and discuss how these characteristics may influence the future model design.

How to cite: Stanisławska, K. and Rögnvaldsson, Ó.: AI model in the real world - analysis of the operational performance of a high-resolution AI weather model for Iceland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18305, https://doi.org/10.5194/egusphere-egu26-18305, 2026.

EGU26-18585 | ECS | Posters on site | AS1.2

Real-Time Solar Irradiance Nowcasting for Renewable Energy Forecasting over Western India 

Sheetal Garg, Subimal Ghosh, Raghu Murtugudde, and Biplab Banerjee

The global transition toward low-carbon energy systems has increased the reliance on renewable energy sources and driven solar power to become a key component of sustainable electricity generation, thereby increasing the importance of accurate irradiance forecasting. As solar penetration grows, power system operations increasingly depend on reliable short-term forecasts to support grid balancing, reserve allocation, and real-time decision-making. Global Horizontal Irradiance (GHI) represents the integrated influence of atmospheric conditions and cloud processes on surface solar radiation and governs short-term variability in photovoltaic power output. However, rapid cloud evolution introduces strong spatiotemporal variability in GHI, making accurate prediction at sub-hourly lead times a persistent challenge for short-term solar forecasting. In this study, we develop a real-time nowcasting system to predict GHI over the western region of India at 15-minute resolution with effective lead times of up to 2 hours. The system is based on a convolutional long short-term memory (ConvLSTM) model that learns spatiotemporal cloud–radiation relationships from high-frequency geostationary satellite observations. We utilize INSAT-3DR and INSAT-3DS products obtained from the MOSDAC archive, which provide continuous monitoring of cloud evolution over the region. The nowcasting framework is implemented using routinely available satellite observations and is evaluated over a large spatial domain covering western India, a region characterized by strong seasonal variability and diverse cloud regimes associated with pre-monsoon, monsoon, and post-monsoon periods. The results demonstrate consistent performance across seasons and show that the system captures the mean diurnal evolution of GHI with stable skill during daytime solar-active periods. Evaluation results indicate mean absolute errors of approximately 60 W m-2 for 1–2 hour lead times and 72 W m-2 for 2–3 hour lead times, corresponding to about 7–12 % of typical daytime GHI under moderate to high irradiance conditions. Overall, this work demonstrates the feasibility of satellite-driven deep learning systems for real-time GHI nowcasting and highlights the potential of integrating geostationary satellite observations and spatiotemporal learning models to support renewable energy forecasting and real-time grid decision-making in regions with high and growing solar power penetration.

How to cite: Garg, S., Ghosh, S., Murtugudde, R., and Banerjee, B.: Real-Time Solar Irradiance Nowcasting for Renewable Energy Forecasting over Western India, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18585, https://doi.org/10.5194/egusphere-egu26-18585, 2026.

EGU26-18808 | ECS | Posters on site | AS1.2

Random forest based precipitation nowcasting for Dakar  

Mai-Britt Berghoefer, Jan O. Haerter, and Diana L. Monroy

Approximately 90% of the total precipitation in Senegal is produced by convective storms. The most intense rainfall events are associated with mesoscale convective systems (MCSs), frequently producing high-intensity rainfall that triggers pluvial flooding. Flood vulnerability is particularly high in the Greater Dakar area due to surface sealing and high population exposure. Timely and reliable short-term precipitation forecasts are therefore essential for effective early warning systems and flood risk reduction.

Precipitation nowcasting aims to describe the current atmospheric state and predict weather evolution at short lead times using real-time observations. The quality and availability of input data are key factors determining the nowcasting performance. In this study, three main data sources are employed: (i) in-situ observations from the High-resolution weather observations East of Dakar (DakE) station network, (ii) satellite-based products such as cloud-top temperature (CTT) from EUMETSAT and precipitation estimates from the Integrated Multi-satellitE Retrievals for GPM (IMERG) algorithm provided by NASA, and (iii) modeled data from the Weather Research and Forecasting (WRF) model.

The objective of this project is to identify a suitable nowcasting approach while weighing the strengths and limitations of the available data sources. Extrapolation-based methods, such as optical-flow techniques implemented in the pySTEPS library, estimate future precipitation by extrapolating observed patterns under the assumption of steady system evolution. These approaches perform well for large, long-lived convective systems, but they are unable to predict convective initiation, decay, and growth. Their applicability is further limited by the temporal resolution and detection uncertainties of the available satellite-based precipitation products identified in comparisons with station observations.

To address these limitations, a machine-learning-based nowcasting framework is developed, primarily relying on the high-temporal-resolution DakE station data to accurately capture atmospheric boundary conditions. Given the limited time span of data collection and the high predictor dimensionality, a Random Forest model was chosen as a robust approach. To mitigate challenges like zero inflation and the underestimation of extreme events, a two-step model architecture is developed: in a first step, a classification forest (I) is used to determine precipitation occurrence and the duration of the predicted event in the lead time horizon. If precipitation is expected, the model is coupled to a regression forest (II) that returns the rainfall intensity of the detected event. Future work will assess potential performance improvements from incorporating CTT-satellite and WRF-modeled data using feature importance analysis, which can also inform the placement of hypothetical new automatic weather stations.

 

 

How to cite: Berghoefer, M.-B., Haerter, J. O., and Monroy, D. L.: Random forest based precipitation nowcasting for Dakar , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18808, https://doi.org/10.5194/egusphere-egu26-18808, 2026.

EGU26-20013 | Orals | AS1.2

Forecast-in-a-Box: AI weather forecasting, easy to run and simple to deploy 

Corentin Carton de Wiart, Harrison Cook, Vojtech Tuma, Jenny Wong, Håvard Alsaker Futsæter, Lene Østvand, Vegard Bønes, Børge Moe, Jørn Kristiansen, James Hawkes, Irina Sandu, and Tiago Quintino

Traditional weather forecasting relies on large scale numerical simulations that run on high-performance computing systems. These methods require substantial computational resources, involve complex workflows, and generate large volumes of data that often exceed individual user needs. Forecast-in-a-Box leverages advances in data-driven modelling to greatly reduce computational and energy costs while delivering tailored forecast products directly to users. Partly funded from the European Commission’s Destination Earth initiative, it packages the entire forecasting chain into a simple and user-friendly application. Built on the open-source Anemoi1 and Earthkit2 projects, it offers a reproducible and modular environment that integrates data access, model execution, and visualisation. This enables accurate forecasts that can be run locally on user desktops, on premise computing infrastructure, or in the cloud.

The approach is being evaluated through a World Meteorological Organization (WMO) Integrated Processing and Prediction System (WIPPS) pilot project led by the Norwegian Meteorological Institute (MET Norway). In this project, a fully packaged forecasting system based on affordable hardware is provided to the Malawi Department of Climate Change and Meteorological Services (DCCMS). The forecasting system is driven by Forecast-in-a-Box and leverages MET Norway’s Bris3 model (Norwegian word for “light wind), a high-resolution data driven weather forecasting model built using the Anemoi framework. The solution is designed to be largely self-contained, with the only external dependency being the retrieval of ECMWF analysis dataset for forecast initialisation.

1https://anemoi.readthedocs.io/en/latest/

2https://earthkit.ecmwf.int

3https://lumi-supercomputer.eu/data-driven-weather-forecasting-model/

How to cite: Carton de Wiart, C., Cook, H., Tuma, V., Wong, J., Futsæter, H. A., Østvand, L., Bønes, V., Moe, B., Kristiansen, J., Hawkes, J., Sandu, I., and Quintino, T.: Forecast-in-a-Box: AI weather forecasting, easy to run and simple to deploy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20013, https://doi.org/10.5194/egusphere-egu26-20013, 2026.

EGU26-112 | ECS | Orals | NP6.6

Lagrangian methods in 2D annular Rayleigh-Bénard convection 

Luis Álamo, Jezabel Curbelo, and Kathrin Padberg-Gehle

In this project, we approach convective instabilities from the perspective of dynamical systems theory, as we seek to identify structures that organize the global and long-term behavior of a system. Lagrangian Coherent Structures (LCSs) are patterns in fluid flows delineating regions that share a certain notion of material coherence, shape global transport and act as mixing barriers [5]. Thus, characterizing these objectively defined structures allows us to gain new insight into how certain invariant manifolds have a fundamental impact on transport and mixing processes in complex natural environments.

On the other hand, thermal convection turns out to be a fundamental process in geophysical and astrophysical flows by driving large amounts of materials through plumes that allow physical processes to be in constant renewal. Examples are convective cores in massive stars and the interior of planets [1]. It also happens to be a crucial driver of turbulence in even more complicated systems, such as accretion disks [8].

To this end, we present an analysis of coherent structures in convective flows in a particularly unexplored geometry: a 2D annulus under the action of a radial inwardly increasing gravity contribution, g∝1/r (r denotes radius). As disks in astrophysical settings are often modeled as rotating concentric cylinders with small height-to-radius ratio, this simple 2D model allows us to make a fairly global picture of the 3D case with reduced computational cost. Thus, we perform hydrodynamic simulations using spectral tau methods via open-source software Dedalus3 [4]. Equipped with a set of tracer trajectories, we implement different (but complementary) coherent structures approaches, namely objective geometrical techniques such as Finite-Time Lyapunov Exponents (FTLE) and Lagrangian-Averaged Vorticity Deviation (LAVD) [6-7] as well as network-based methods [8].

In this presentation, we will discuss our latest results combining these approaches. We will also make some useful comparisons with [2-3] that complement their Eulerian study in the same geometry.

References

[1] E.H. Anders et al., The Astrophysical Journal, 926, 169 (2022).

[2] A. Bhadra, O. Shiskina, X. Zhu, Journal of Fluid Mechanics, 999, R1 (2024).

[3] A. Bhadra, O. Shiskina, X. Zhu, International Journal of Heat and Mass Transfer, 241, 126703 (2025).

[4] K.J. Burns, G.M. Vasil, J.S. Oishi, D. Lecoanet, B.P. Brown, Phys. Rev. Res., 2, 23–68 (2020).

[5] G. Haller and G. Yuan, Physica D: Nonlinear Phenomena, 147, 352-370 (2000)

[6] G. Haller, Journal of the Mechanics and Physics of Solids, 86, 70–93 (2015).

[7] G. Haller, A. Hadjighasem, M. Farazmand, F. Huhn, Journal of Fluid Mechanics, 795,

136–173 (2016).

[8] C. Schneide, P.P. Vieweg, J. Schumacher, K. Padberg-Gehle, Chaos, 32, 013123 (2022).

[9] R. Teed and H. Latter, MNRAS, 507, 5523-5541 (2021).

How to cite: Álamo, L., Curbelo, J., and Padberg-Gehle, K.: Lagrangian methods in 2D annular Rayleigh-Bénard convection, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-112, https://doi.org/10.5194/egusphere-egu26-112, 2026.

Ocean currents transport material like nutrients, plankton and plastic over the globe. The most natural way to study these transport pathways and the connections between ocean basins is by using trajectories, computed by simulating virtual Lagrangian particles in fine-resolution ocean models.

In this presentation, I will show how my team uses our open source parcels-code.org framework to simulate the dispersion of virtual plastic particles by the three-dimensional ocean flow. I will discuss how we develop new parameterizations for subgrid-scale transport processes of buoyant plastics; and compare these parameterizations to field measurements.

I will particularly focus on how we combine the resulting dispersion maps with estimates of plastic pollution sources and then apply Bayesian inference techniques to find the most likely sources for heavily polluted locations.

While our application is plastic pollution in the ocean, the framework could be applied in other geophysical contexts where the sources of a signal in a complex Lagrangian transport process have to be determined, from air pollution tracking to glaciological proxy reconstruction.

How to cite: van Sebille, E.: Combining Lagrangian simulations and Bayesian inference for source attribution of ocean plastic pollution, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1946, https://doi.org/10.5194/egusphere-egu26-1946, 2026.

EGU26-4256 | ECS | Orals | NP6.6

Vertical distribution of weakly inertial, quasi-neutrally buoyant particles in a convective ocean mixed layer 

Luz Andrea Silva Torres, Stefano Berti, and Enrico Calzavarini

Microplastic pollution is one of the major threats to ocean health. However, the processes governing the transport and redistribution of microplastics remain poorly understood due to the interaction of multiple physical mechanisms at different scales  We investigate the vertical transport and concentration of quasi-neutrally buoyant microplastics by direct numerical simulations of small inertial particles in an inhomogeneous turbulent flow. An idealized two-dimensional convective mixed-layer model reproduces some relevant features of the upper ocean: at the surface, a well-mixed region where temperature and density are nearly homogeneous, and a lower region of weak mixing and gravity waves with strong temperature and density gradients. The dynamics of these inertial particles in both regions are analyzed using a simplified model derived from the Maxey-Riley-Gatignol equation. The model assumes particle density equal to a reference fluid density at a given depth, with density variations only affecting buoyancy (i.e., the Boussinesq approximation). Our results show that temperature differences along Lagrangian paths determine whether particles settle at specific depths or remain near the surface. The observed vertical concentration profiles in the thermocline are explained using a discrete particle framework based on a stochastically forced wave–driven relaxation model. Particle accumulation occurs preferentially near specific depths where internal gravity wave signatures are detected through oscillations of the local isopycnal structure. In the proposed description, these wave-induced fluctuations imprint a structured modulation of the concentration profile, while turbulent fluctuations are represented as a white-noise forcing that accounts for particle spreading around the accumulation depths. The relative importance of wave-driven relaxation and turbulent diffusion varies with depth, reflecting the anisotropic and inhomogeneous nature of the stratified flow. This approach consistently reveals that, while gravity has a pivotal role on particle transport and accumulation, the fluid’s eddy diffusivity can also have non-negligible effects on the spreading of particles, depending on the physical properties of the latter.

How to cite: Silva Torres, L. A., Berti, S., and Calzavarini, E.: Vertical distribution of weakly inertial, quasi-neutrally buoyant particles in a convective ocean mixed layer, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4256, https://doi.org/10.5194/egusphere-egu26-4256, 2026.

EGU26-7025 | ECS | Orals | NP6.6

Mesoscale fronts and eddies shape neon flying squid distribution through effective transport 

Zixuan Niu, Zhaohui Chen, Wei Yu, and Jia-Zhen Wang

Mesoscale oceanic fronts and eddies form coherent structures that regulate transport, retention, and mixing in the upper ocean, yet how their internal physical and biogeochemical structure shapes the distribution of mobile predators remains poorly understood. Here we adopt an active Lagrangian perspective to investigate the distribution of neon flying squid (Ommastrephes bartramii) using a decade-long fisheries dataset from the Northwest Pacific, combined with mesoscale diagnostics and Biogeochemical Argo observations.

Across multiple frontal systems, squid catches exhibit a robust cross-frontal asymmetry: catches are on average 1.6-fold higher on the warm side, with an optimal fishing offset of ~10 km toward warmer waters. This pattern arises from behaviorally mediated effective transport across a sloping frontal interface. Squid undergo diel vertical migration, occupying colder subsurface layers during daytime and ascending toward frontal zones at night. Because frontal surfaces tilt downward toward the warm side, subsurface squid habitats are systematically displaced relative to surface frontal indicators and fishing locations, producing a persistent warm-side bias without invoking passive advection.

In mesoscale eddies, squid distributions display a contrasting but complementary structure. Squid preferentially aggregate near the cores of warm-core eddies, whereas in cold-core eddies they are predominantly distributed along the outer periphery. Biogeochemical Argo float observations reveal that these patterns are closely linked to differences in the vertical structure of temperature and dissolved oxygen, which modulate habitat depth and suitability. Warm-core eddies provide vertically expanded, oxygen-rich habitats conducive to retention near the eddy center, while cold-core eddies constrain suitable habitat to peripheral regions.

Together, these results demonstrate how mesoscale coherent structures—fronts acting as transport barriers and eddies acting as retentive or exclusionary features—interact with active predator behavior to shape asymmetric spatial distributions. This study highlights how effective transport and mixing of mobile marine organisms can be interpreted within a Lagrangian framework integrating physical structure, biogeochemical environment, and behavioral dynamics.

How to cite: Niu, Z., Chen, Z., Yu, W., and Wang, J.-Z.: Mesoscale fronts and eddies shape neon flying squid distribution through effective transport, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7025, https://doi.org/10.5194/egusphere-egu26-7025, 2026.

Rotation and turbulence jointly shape transport and mixing in jet-like flows, from boundary currents to atmospheric plumes. Even under weak rotation (Rossby number O(1)), particle spreading can become strongly inhomogeneous because material barriers reorganize pathways and constrain exchange across the turbulent–non-turbulent interface. Here we use a laboratory horizontal jet to quantify how rotation regulates Lagrangian dispersion in distinct jet sub-regions (core versus edges) and to link the observed trends in dispersion and diffusivity to the geometry of transient attracting barriers.

We analyse three experiments (datasets previously presented in De Serio et al., 2021): a non-rotating reference case (EXP14) and two rotating cases with increasing rotation rate (EXP15 and EXP16). Experiments were conducted using a turbulent, non-buoyant jet released horizontally into ambient water (initial diameter d=0.08m, exit velocity u=1.14m/s). Planar PIV velocity fields are integrated to compute Lagrangian trajectories of numerical neutrally buoyant particles. We evaluate single-particle absolute dispersion A(t) and direction-dependent absolute diffusivities K(t). 

We also diagnose barrier-structured transport without time-integration, using Transient Attracting Profiles (TRAPs), an instantaneous diagnostic of the most attracting regions of the flow derived from local minima of the strain-rate tensor (Serra et al., 2020; Kunz et al., 2024). TRAPs mark hyperbolic skeletons of maximal compression on the measurement plane, predicting where tracers accumulate and where strong stretching develops. In our jet, TRAPs provide a compact geometric context for interpreting when and where lateral spreading is inhibited (reduced A or analogously K) or promoted (enhanced stretching and growth of A and K).

Across all cases, we note that A(t) exhibits an initial ballistic regime consistent with inertial short-time behaviour. Rotation then introduces a clear, region-dependent ordering. In the jet core, focusing on intermediate dispersion values (i.e. structures of order 10–100 cm), these levels are reached first in EXP14 (no rotation), then in EXP15, and last in EXP16, demonstrating that core dispersion decreases as rotation increases. Consistently, the growth of K(t) is progressively suppressed under stronger rotation, indicating stabilization and more coherent pathways. At the jet edges, the rotating cases show the same ordering, so that stronger rotation implies lower dispersion. In contrast, without rotation (EXP14) edge-region dispersion is minimal. Interpreted through TRAP geometry, stronger rotation favours tighter attracting pathways and enhanced accumulation along compressive skeletons, reducing cross-interface wandering and lowering edge-region diffusivities, while non-rotating edges remain weakly dispersive because velocities are small and entrainment is limited.

Overall, rotation reduces dispersion in both core and edge regions, but through distinct mechanisms: stabilization driven by the Rossby number in the core and entrainment-mediated limitation at the edges, with TRAPs offering an immediate geometric interpretation of the observed A and K trends.

References

De Serio et al. 2021: https://doi.org/10.1007/s00348-021-03297-2.

Serra et al. 2020: https://doi.org/10.1038/s41467-020-16281-x.

Kunz et al. 2024: https://doi.org/10.5194/os-20-1611-2024.

How to cite: De Serio, F.: Rotation–entrainment control of Lagrangian dispersion in a turbulent horizontal jet: core–edge contrasts and transient attracting barriers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7326, https://doi.org/10.5194/egusphere-egu26-7326, 2026.

EGU26-9297 | ECS | Posters on site | NP6.6

Time-variable flux of sinking aggregates to the deep ocean: Hybrid Eulerian-Lagrangian model 

Seongbong Seo, Vladimir Maderich, Kateryna Kovalets, Igor Brovchenko, and Kyeong Ok Kim

The descending flux of organic particles, formed in the euphotic layer of the ocean, is a key mechanism for delivering carbon and nutrients into the deep ocean layers. Our study aimed to enhance the model and numerical Eulerian-Lagrangian algorithm developed by Maderich et al. (2025) so that it can consider the time-dependent dynamics of aggregate flux and account for ballast minerals (silicate and calcium carbonate) in aggregate sinking. In the algorithm, the Euler equations were solved for spectral concentrations of aggregate components with different sizes, while the Lagrangian equations were solved for depth and sizes of individual aggregates. Novel analytical unsteady solutions of the system of one-dimensional equations in the Eulerian framework for the particulate organic matter (POM) concentration and the Lagrangian framework for the particle mass and depth for constant and age-dependent degradation were compared with numerical solutions. The impact of a bloom event on POM profile variability was simulated using the developed numerical algorithm.

 

Vladimir Maderich, Igor Brovchenko, Kateryna Kovalets, Seongbong Seo, and Kyeong Ok Kim (2025). Simple Eulerian–Lagrangian approach to solving equations for sinking particulate organic matter in the ocean. Geosci. Model Dev., 18, 7373–7387

How to cite: Seo, S., Maderich, V., Kovalets, K., Brovchenko, I., and Kim, K. O.: Time-variable flux of sinking aggregates to the deep ocean: Hybrid Eulerian-Lagrangian model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9297, https://doi.org/10.5194/egusphere-egu26-9297, 2026.

EGU26-10343 | ECS | Posters on site | NP6.6

Lagrangian evaluation of surface transport around the Canary Islands using drifter observations and OpenDrift simulations 

Jacob S. Torres-Ojeda, Ángel Rodríguez-Santana, Antonio J. Gonzáles-Ramos, Ana M. Mancho, Alejandro Garcia-Mendoza, Giovanny A. Cuervo-Londoño, Luis Yubero, and Ángeles Marrero-Díaz

The prediction of ocean surface trajectories remains a key challenge in coastal and island-influenced regions, were strong spatial variability limits model skill. Previous Lagrangian studies have shown the usefulness of drifter observations to assess trajectory predictability and to compare different sources of surface currents (e.g. Dagestad and Röhrs, 2019). In this context, Lagrangian approaches provide a direct and observation-based framework to evaluate surface transport.
This study assesses surface transport predictability around the Canary Islands using trajectories from two surface drifters (CODE/Davis type, drogued at 1 m depth) and numerical simulations performed with the OpenDrift framework (Dagestad et al., 2018). Simulations are forced with surface currents from the Iberia–Biscay–Ireland (IBI) regional ocean model distributed by the Copernicus Marine Environment Monitoring Service (CMEMS), and, where available, from the high-resolution coastal forecasting system SAMOA (Sotillo et al., 2019), operationally implemented for Spanish ports. Wind forcing is provided by ERA5 atmospheric fields, and wave-induced Stokes drift is included using IBI wave products from CMEMS.
From each observed drifter position, short-term forward simulations are performed to predict the subsequent drifter location. Model performance is quantified through the separation distance between simulated and observed positions, allowing a direct comparison of transport skill between different current products and forcing configurations.
The oceanic and atmospheric datasets used in this study correspond to operational or near-real-time products rather than fully consolidated reanalysis, reflecting realistic conditions for trajectory forecasting applications. The results reveal pronounced spatial and temporal variability in the separation between modeled and observed positions, with the relative performance of SAMOA and IBI depending on location and conditions, and neither consistently outperforming the other. While further improvements in transport predictability are expected once consolidated reanalysis products become available, the present results already provide a robust assessment of Lagrangian model skill under operational conditions.


Acknowledgments:
This work was supported by the projects SIRENA and SIRENA 2, funded by the collaboration of the Biodiversity Foundation of the Ministry for the Ecological Transition and the Demographic Challenge, through the Pleamar Program, and are co-financed by the European Union through the EMFAF (European Maritime, Fisheries and Aquaculture Fund).


References:
Dagestad, K.-F., Röhrs, J., Breivik, Ø., & Ådlandsvik, B. (2018): OpenDrift v1.0: a generic framework for trajectory modelling, Geoscientific Model Development, 11, 1405–1420, https://doi.org/10.5194/gmd-11-1405-2018
Dagestad, K.-F., & Röhrs, J. (2011): Prediction of ocean surface trajectories using satellite derived vs. modeled ocean currents, Ocean Modelling. https://doi.org/10.1016/j.rse.2019.01.001
Sotillo, M. G., Cerralbo, P., Lorente, P., Grifoll, M., Espino, M., Sanchez-Arcilla, A., & Álvarez-Fanjul, E. (2019): Coastal ocean forecasting in Spanish ports: the SAMOA operational service, Journal of Operational Oceanography, 13, 37–54, https://doi.org/10.1080/1755876X.2019.1606765
Copernicus Marine Environment Monitoring Service (CMEMS): IBI Ocean Currents Product, https://doi.org/10.48670/moi-00027
Copernicus Marine Environment Monitoring Service (CMEMS): IBI Stokes Drift Product, https://doi.org/10.48670/moi-00025
Hersbach, H. et al. (2020): ERA5 global reanalysis, Copernicus Climate Change Service (C3S), https://doi.org/10.24381/cds.adbb2d47

How to cite: Torres-Ojeda, J. S., Rodríguez-Santana, Á., Gonzáles-Ramos, A. J., Mancho, A. M., Garcia-Mendoza, A., Cuervo-Londoño, G. A., Yubero, L., and Marrero-Díaz, Á.: Lagrangian evaluation of surface transport around the Canary Islands using drifter observations and OpenDrift simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10343, https://doi.org/10.5194/egusphere-egu26-10343, 2026.

We apply  generalized spectral clustering methods to the global Argo dataset and compare the identified clusters with those obtained from established dynamical systems approaches, including finite-time Lyapunov exponents (FTLEs), Lagrangian-averaged vorticity deviation (LAVD), encounter volume, and a newly introduced tool— retention volume.

Spectral clustering provides a powerful framework for identifying Lagrangian coherent clusters from particle trajectories, grouping together trajectories that evolve similarly while remaining distinct from others. Traditionally, spectral clustering relies on physical proximity to define similarity between particles. Here, we extend this approach by incorporating additional oceanographic properties—such as temperature, salinity, density, and spiciness—into the similarity measure. This generalization allows us to detect coherent water masses that are not only spatially coherent but also share key physical characteristics.

Our results highlight the potential of the generalized spectral clustering method, combined with Argo measurements, to provide new insights into ocean transport and water mass transformations.

How to cite: Curbelo, J. and Rypina, I. I.: Application of a generalized spectral clustering method for characterizing water masses using Argo floats, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14129, https://doi.org/10.5194/egusphere-egu26-14129, 2026.

EGU26-17328 | ECS | Posters on site | NP6.6

Lagrangian Dynamics of Anisotropic Crystals in Vigorous Mantle Convection 

Raaghava Murthi, Anu V S Nath, and Anubhab Roy

The dynamics of anisotropic crystals in cellular convective flows are critical for understanding the development of seismic anisotropy and chemical mixing in the Earth's mantle. In this study, we investigate the transport and orientation of slender rigid inclusions, proxies for anisotropic minerals such as olivine, using a Lagrangian framework. The crystals are modelled as inertialess rod-like tracers, with translational motion derived by averaging the background flow velocity along the crystal's major axis, and rotational dynamics determined by the moment of the background velocity field evaluated along the length. Unlike passive point tracers, these extended objects exhibit intrinsically coupled translation and rotation, resulting in preferred orientations (LPO) that depend sensitively on both the convective flow structure and crystal aspect ratio.

To benchmark the model, crystal dynamics are first examined in idealised laminar flows relevant to mantle kinematics, including two-dimensional Taylor–Green cellular flow and eigenmodes of Rayleigh–Bénard convection. These configurations allow for the analysis of crystal trajectories, stability near stagnation points, and the influence of density contrasts (settling) on crystal residence times. The study is then extended to vigorous, chaotic thermal convection by generating high-Rayleigh-number flows using direct numerical simulations of the Boussinesq-approximated Navier–Stokes equations. Crystals are introduced into the statistically steady flow field to simulate entrainment and mixing processes.

Confinement effects, representing lithospheric boundaries or phase transitions, are modelled using a soft-wall collision scheme, while periodic boundary conditions mimic the lateral extent of the mantle. We quantify crystal dispersion and alignment over a range of geophysical parameters, exploring variations in the Rayleigh number and crystal geometry. Statistical analyses focus on long-time orientation distribution functions (ODFs) and dispersion rates. Our results reveal how convective vigour and coherent structures (e.g., plumes and downwellings) jointly govern the evolution of fabric in the mantle, offering a controlled framework for interpreting seismic anisotropy in thermally driven flows.

How to cite: Murthi, R., V S Nath, A., and Roy, A.: Lagrangian Dynamics of Anisotropic Crystals in Vigorous Mantle Convection, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17328, https://doi.org/10.5194/egusphere-egu26-17328, 2026.

The ocean biological carbon pump transfers particulate organic matter (POM) from surface waters to the deep ocean, playing a key role in long-term sequestration of organic matter. Small-scale turbulence and stratification strongly influence particle sinking, yet these processes are poorly represented in global models, which rely on simplified parameterizations.

We investigate these effects using high-resolution direct numerical simulations (DNS) of stratified turbulence, designed to capture small-scale ocean dynamics, coupled with a Lagrangian inertial particle model. By resolving turbulent structures and particle–fluid interactions, we aim to quantify how turbulence intensity, stratification, and particle properties control sinking velocities and export efficiency. Multiple particle types are tracked under ocean-relevant conditions, constrained using oceanographic observations and reanalysis data to provide realistic ranges for turbulence, stratification, and vertical shear.

To bridge microscale processes to large-scale modeling, we incorporate DNS-derived insights into climate simulations using the Earth System Model EC-Earth, a fully coupled atmosphere–ocean configuration. The ocean and its biogeochemistry are simulated with NEMO-PISCES, and the atmosphere with OIFS. This approach allows us to assess how unresolved turbulence and particle dynamics affect particulate export at global scales. By combining turbulence-resolved Lagrangian simulations with global climate experiments, this work aims to reduce uncertainties in particle transport and improve understanding of biogeochemical microscale processes and their climate feedbacks. Simulation data and tools will be openly available to enable further research on microscale ocean transport processes and their representation in global climate and ocean models.

How to cite: Sozza, A. and Davini, P.: Towards a Lagrangian-informed representation of ocean particulate export: from small-scale turbulence to climate models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18046, https://doi.org/10.5194/egusphere-egu26-18046, 2026.

EGU26-19360 | ECS | Orals | NP6.6

Tracing the toxic bloom: Dispersion, impacts, and perspectives of Prymnesium parvum in the Oder Lagoon 

Bruna de Ramos, Siren Rühs, Clemens Engelke, Thomas Neumann, and Gerald Schernewski

Harmful Algal Blooms (HABs) caused by the haptophyte Prymnesium parvum represent an ecological and socio-economic threat in brackish waters worldwide. In summer 2022, a catastrophic bloom in the Oder River (Germany–Poland) caused mass fish kills (~360 t). The Oder River discharges into the Oder (Szczecin) Lagoon, a region with fisheries tradition and growing importance for tourism and recreation. Understanding how the bloom affected the lagoon is important for future risk assessment.

We combined long-term (1972-2024) phytoplankton monitoring data from Polish and German environmental authorities, high-resolution (200m horizontal grid from MOM – Modular Ocean Model) hydrodynamic modeling, and Lagrangian particle tracking (Parcels framework) to (1) assess historical occurrence of Prymnesiophyceae in the lagoon, (2) simulate decay and transport of the 2022 bloom from the river into the lagoon, (3) evaluate connectivity between different regions in the lagoon and the Baltic Sea, and (4) generate ecological and socio-economic risk maps.

Phytoplankton time series show that Prymnesiophyceae have been present in the lagoon since 2007, with the higher abundance (~ 100 million cells L-1) recorded in July 2022, in the German side of the lagoon. Regarding the 2022 bloom, we released virtual water parcels with a P. parvum initial abundance of 150 million cells L-1 from the river mouth. We started the simulation on July 15 2022, applying different decay scenarios (no decay, 5-day and 10-day half-life). Particles were tracked for 30 days to identify hotspots and connectivity.

Even under slow decay, all water parcels remained in the Polish sector (Wielki Zalew), affecting beaches like Plaża w Czarnocinie about 6km from the river mounth. Connectivity matrix based on releasing water parcels from German and Polish sides supported the low connectivity between lagoon portions and the Baltic in a one-month time frame. This suggests that P. parvum observed on the German side in 2022 likely originated from local or previously established populations rather than direct influence by the bloom event.

We integrated modeled bloom dispersion with ecological subjects (key fish species and habitats) and socio-economic features (fisheries harbors, bathing beaches) to produce risk maps. Polish side areas were more affected from the bloom regardless the decay rate and presented higher risk.

However, in future scenarios, increasing drought frequency may support long-term risk of toxic algae blooms in the Oder River. Monitoring identifying Prymnesiophyceae and our risk maps could serve as important management information. Also, our particle tracking applied to different hydrodynamic conditions could help to improve the understanding of risk areas.

How to cite: de Ramos, B., Rühs, S., Engelke, C., Neumann, T., and Schernewski, G.: Tracing the toxic bloom: Dispersion, impacts, and perspectives of Prymnesium parvum in the Oder Lagoon, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19360, https://doi.org/10.5194/egusphere-egu26-19360, 2026.

EGU26-21101 | ECS | Orals | NP6.6

Tracking Industrial Emissions and Odor Nuisance through Integrated Modeling and Citizen Reporting 

Giorgio Veratti, Anna Abita, Nicolò Tirone, Giorgio Resci, Giovanni Guidi, Paolo Bonasoni, and Tony Christian Landi

The management of air quality in residential areas adjacent to large industrial hubs requires addressing two distinct yet overlapping challenges: monitoring pollutants with health implications and mitigating odor nuisances that significantly degrade quality of life. This study presents a multidisciplinary, integrated system designed to track, quantify and attribute these atmospheric impacts in one of Europe’s largest coastal petrochemical complexes. In the industrial area of Syracuse Province (Sicily, Italy), the emissions from refineries and port activities are a persistent source of both health concerns and community complaints. The NOSE (Network for Odour SEnsitivity) system has been operational since 2019 across the municipalities of Melilli, Priolo, Augusta and Siracusa, enabling citizens to report, via a dedicated web-app, the intensity and specific characteristics of odor episodes. In this framework, we developed an experiment based on three integrated pillars: a network of air quality and meteorological monitoring stations, the GRAMM-GRAL Lagrangian dispersion model and the data collected by the NOSE system. To address the frequent underestimation of the emissions in standard inventories, a Bayesian inversion framework was implemented to optimize prior emission estimates of benzene (C6H6), toluene (C7H8) and hydrogen sulphide (H2S). Given the limitations of Lagrangian models in representing the photochemistry of complex volatile organic compounds, C6H6 and H2S were used as conservative tracers and proxies for highly odorant non-methane hydrocarbon mixtures typically emitted by refinery processes.
Our findings demonstrate that the inversion procedure substantially improved dispersion model performance. The use of posterior emissions reduced the average Root Mean Square Error across all stations from 1.69 to 0.78 µg m-3 for C6H6, from 2.46 to 0.76 µg m-3 for C7H8, and from 8.1 to 0.81 µg m-3 for H2S. Correspondingly, the average Pearson correlation coefficient increased from 0.25 to 0.67 for C6H6 and C7H8, and from near-zero values to 0.45 for H2S. Finally, we compared forward simulations using posterior emissions with spatio-temporal clusters of odor nuisance reports submitted by citizens. These results suggest that two major coastal refineries are the primary contributors to regulated pollutant concentrations and citizen-reported odor impacts. This integrated system, which combines citizen reporting, Lagrangian dispersion modeling and Bayesian inversion, provides local authorities with a powerful tool for identifying high-impact sources and developing targeted strategies for health protection and odor mitigation.

How to cite: Veratti, G., Abita, A., Tirone, N., Resci, G., Guidi, G., Bonasoni, P., and Landi, T. C.: Tracking Industrial Emissions and Odor Nuisance through Integrated Modeling and Citizen Reporting, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21101, https://doi.org/10.5194/egusphere-egu26-21101, 2026.

EGU26-21936 | ECS | Orals | NP6.6

An Integrated clear air turbulence scheme for the FLEXPART model 

Lokahith Narendra Agasthya and Andreas Stohl

Atmospheric turbulence above the planetary boundary layer (PBL) plays a critical role in the vertical and horizontal mixing of aerosols and trace gases. In the troposphere, such turbulence is highly intermittent and primarily associated with jet stream boundaries and planetary-scale waves, while in the stratosphere it is strongly modulated by the quasi-biennial oscillation. Owing to the long residence times of air masses in the stratosphere, vertical mixing across the tropopause and within the stratosphere is a key process controlling stratospheric composition. Accurate representation of stratospheric transport is also essential to understand the dispersion and lifetime of sulphur aerosols injected for potential solar radiation management applications.

Lagrangian atmospheric transport models commonly represent turbulent mixing using spatially and temporally constant diffusion coefficients, despite the inherently intermittent nature of turbulence in the free atmosphere. In this study, we implement a time- and space-dependent turbulent mixing scheme in the FLEXPART model, based on local diffusion coefficients derived from the Richardson number. This parameterization is consistent with the scheme used natively in the IFS model to represent turbulent exchange above the PBL.

Using a suite of sensitivity experiments, we investigate the impact of intermittent turbulent mixing on the distribution of trace gases in both the troposphere and stratosphere. Our approach provides a unified representation of turbulence from the boundary layer to the uppermost model levels, enabling a more physically consistent treatment of atmospheric mixing across dynamical regimes.

How to cite: Agasthya, L. N. and Stohl, A.: An Integrated clear air turbulence scheme for the FLEXPART model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21936, https://doi.org/10.5194/egusphere-egu26-21936, 2026.

EGU26-22376 | ECS | Orals | NP6.6

Priority conservation areas based on plankton particle trajectories as an alternative to marine protected areas 

Oscar Julian Esteban-Cantillo, Damien Eveillard, Sabrina Speich, and Roberto Casati

Ecological modelling has enhanced our understanding of ecosystems and biodiversity, and it has been widely used in policy decision-making. Strengthening our ability to represent ecosystems and their interactions with human activities is a global priority for achieving conservation goals. However, most existing spatial conservation frameworks rely on staticMarine Protected Areas (MPAs), defined by fixed geographic boundaries and invariant management rules that do not account for the strong temporal variability, circulation-driven connectivity, and climate-induced shifts that characterize marine ecosystems. As a result, static MPAs may fail to consistently protect key ecological processes, particularly in pelagic systems where biological organization is shaped by moving water masses. One way to address this is through the design and implementation of “dynamic” Marine Protected Areas (dMPAs) - areas that shift in space and time based on plankton trajectories, given their ecological importance. The recognition of the importance of marine plankton for human well-being has sparked proposals to prioritize plankton in marine policymaking. Yet scientific investigation into defining species-based areas has not been undertaken, despite their fundamental role in sustaining the oceans and marine life. Our research demonstrates the value of adopting dynamic approaches for conserving marine ecosystems, which are highly variable and interconnected by ocean circulation. Using a Lagrangian particle-tracking framework implemented with OceanParcels, we simulate the transport, retention, and aggregation of planktonic communities by integrating hydrodynamic fields with plankton distribution models. From these simulations, we identify spatiotemporal hotspots of particle aggregation and retention, interpreted as regions of enhanced ecological significance, which we define as Plankton Priority Areas for Conservation (PPACs). By comparing aggregation patterns across winter, spring, summer, and autumn, we identify both seasonal hotspots and areas of persistent retention. To place PPACs in a broader conservation context, we assess their overlap with four complementary indicators - biodiversity distribution, climate resilience, carbon sequestration potential, and ecosystem vulnerability. Our results demonstrate that dynamic, circulation-informed conservation areas can reveal ecologically critical regions that are poorly represented by static MPAs and provide a flexible, scalable complement to existing conservation tools in a changing ocean. 

How to cite: Esteban-Cantillo, O. J., Eveillard, D., Speich, S., and Casati, R.: Priority conservation areas based on plankton particle trajectories as an alternative to marine protected areas, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22376, https://doi.org/10.5194/egusphere-egu26-22376, 2026.

Atmospheric Lagrangian particle dispersion models (LPDMs) are commonly combined with Bayesian inversion/optimization methods to infer emission fluxes across spatial scales from local to global. These tools are central to monitoring greenhouse gases, especially CO₂, CH₄, and N₂O. However, uncertainties in flux estimates arise from multiple sources: prior flux information, representation of the background atmospheric composition, statistical model choices (including hyperparameters and error covariance assumptions), and errors in atmospheric transport. In this presentation, we describe current uncertainty quantification activities linked to ongoing projects (e.g. EYE-CLIMA). We will discuss the use of meteorological ensemble simulations to assess transport related uncertainty and explore connections with dynamical systems tools and common assumptions such as Gaussian errors. Emphasis will be placed on high-resolution transport modelling applications.

How to cite: Pisso, I.: Uncertainties associated with Lagrangian transport in greenhouse gas flux estimates, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22836, https://doi.org/10.5194/egusphere-egu26-22836, 2026.

NP7 – Nonlinear Waves

EGU26-2532 | Posters on site | NP7.1

Macroscopically microstructural effects on wave propagation in highly stressed fractured rocks 

Li-Yun Fu, Haidi Yang, Jianxiong Tang, and Haochen Zheng

Stress-dependent seismic velocities in fractured rocks arise from the coupled deformation of a macroscopically continuous background matrix and stress-sensitive microstructures such as microcracks and aligned fractures. To capture this multi-source nonlinearity together with microstructural size effects, we develop a unified third-order strain-gradient acoustoelastic framework that embeds nonlocal strain-gradient micromechanics into classical acoustoelasticity based on third-order elastic constants, enabling micro–macro coupling through a total strain-energy function. 

We validate the theory using ultrasonic transmission measurements on two artificial sandstones sharing the same background matrix: an intact sample containing native microdefects and a cracked sample with uniformly implanted aligned penny-shaped cracks. Measurements were conducted under dry conditions at 500 kHz with hydrostatic pressure from 5 to 50 MPa, and anisotropic velocities were constrained using propagation directions normal and parallel to the bedding/crack plane. The proposed model reproduces the strongly nonlinear velocity–pressure trends in the low-pressure regime dominated by progressive crack closure, while remaining consistent with the near-linear regime at higher pressure.

A key outcome is a physically interpretable characteristic scale 𝑔 representing an evolving microstructural length associated with stress-driven changes in compliant pore space. We show that 𝑔 exhibits an asymptotic pressure dependence consistent with cumulative compliant-porosity evolution, and that these quantities are systematically correlated. Using effective-medium parameterizations for penny-shaped cracks (Hudson and Padé–Hudson), we further demonstrate that 𝑔2 scales approximately linearly with fracture (crack) porosity across a range of crack aspect ratios and parameter ranges, supporting a robust micro–macro linkage.

These results provide a physics-guided route to connect stress-driven microstructural evolution with macroscopic wave observables, with implications for fracture characterization and seismic monitoring in stressed crustal systems.

How to cite: Fu, L.-Y., Yang, H., Tang, J., and Zheng, H.: Macroscopically microstructural effects on wave propagation in highly stressed fractured rocks, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2532, https://doi.org/10.5194/egusphere-egu26-2532, 2026.

EGU26-9269 | Posters on site | NP7.1

P-wave triggering of periodic fault sliding. Negative friction 

Arcady Dyskin and Elena Pasternak

Sliding of a fault with gouge leads to rotation of gouge particles. Since the particles are not spherical, their rotation in the presence of pressure normal to the fault can exhibit local negative shear stiffness. Another mechanism of local negative shear stiffness is rotations of couples of temporary connected particles. These rotations affect the relation between the shear sliding stress and normal stress creating the effect of apparent friction coefficient, which, in some locations, can become negative [1]. The value (and the sign) of the local stiffness and the apparent friction coefficient depend upon the initial pressure and the stiffness of the surrounding rock. When elastic p-wave approaches a fault in normal direction it causes both normal and shear oscillations of one fault face against the other. If the amplitude of the wave-generated normal oscillations exceeds a certain threshold which depends upon fault and particles’ geometry and rock stiffness, then the shear oscillations reach the negative stiffness stage and become unstable. This leads to unstable periodic fault sliding resulting in seismic events.

The proposed concept will form a basis for developing realistic models of sliding and periodic seismicity of fault with gouge. It will also facilitate developing models of monitoring of fractures affecting thermal spallation mechanics.

Acknowledgement. The authors acknowledge financial support from of the Australian Research Council through project DP250103594.

1. Pasternak, E. and A. Dyskin, 2025. Negative stiffness induced and controlled by constriction. Status Solidi B DOI: 10.1002/pssb.202500428 (in print).

How to cite: Dyskin, A. and Pasternak, E.: P-wave triggering of periodic fault sliding. Negative friction, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9269, https://doi.org/10.5194/egusphere-egu26-9269, 2026.

EGU26-9365 | Posters on site | NP7.1

Mode I fractures with distributed bridges. Scaling and monitoring 

Elena Pasternak and Arcady Dyskin

Traces of Mode I fractures in rocks (cracks in rock samples, hydraulic fractures, magmatic dikes, Mis-Ocean Ridges) are usually not straight; they exhibit interruptions and overlappings [1]. These are 2D features belonging to a particular cross-sectional view. In 3D interruptions and overlappings represent local bridges connecting the opposite sides of the fracture and distributed all over it. These bridges constrict the fracture opening and reduce the values of the stress intensity factor. The dimensions, the number and the geometry of the bridges depend upon the rock structure (at the scale microscopic with respect to the fracture length). Therefore, understanding the effect of bridges on the stress intensity factor can shed light on the rock microstructure. The combined effect of uniformly distributed bridges is accounted for by the introduction of constriction length [1]. As a result, under the given stress the stress intensity factor depends on both the fracture length and the ratio of fracture length to the constriction length.

Fracture propagation is controlled by fracture toughness, which is usually determined by measuring/estimating the fracture length, and the load at which fracture propagates. For this the conventional models neglecting the effect of bridges are employed. This shows a scale effect, the increase of fracture toughness with fracture length [2-5]. We used the model of constricted fracture propagation and found that for each scale there exists a constriction length such that scale effect of fracture toughness disappears and the fracture toughness remains constant.

Determination of constriction length allows more realistic monitoring of fracture growth and provides insight into the rock structure. It will also allow developing a more realistic scaling of fracture growth in strain rock burst and thermal spallation.

Acknowledgement. The authors acknowledge financial support from of the Australian Research Council through project DP250103594.

1. Dyskin, A.V., E. Pasternak, S. Shapiro and A. Bunger, 2025. Scaling laws for hydraulic fractures with constricted opening. Engineering Fracture Mechanics, 327 (2025) 111464.

2. Kobayashi, R., K. Matsuki and N. Otsuka, 1986. 2. Size Effect in The Fracture Toughness of Ogino Tuff. J. Rock Mech. Min. Sci. & Geomech. Abstr. 23, 13-18.

3. Shlyapobersky, J. 1985. Energy analysis of hydraulic fracturing. 26th US Symposium on Rock Mechanics / Rapid City, SD / 26-28 June 1985, 539-546.

4. Delaney, P.T. and D.D. Pollard, 1981. Deformation of host rocks and flow of magma during growth of Minette Dikes and Breccia-bearing intrusions near Ship Rock, New Mexico. Geological Survey Professional Paper 1202, 1-61.

5. Macdonald, K.C., D.S. Scheirer and S.M. Carbotte, 1991. Mid-Ocean Ridges: Discontinuities, segments and giant cracks. Science, 253, 986-994.

How to cite: Pasternak, E. and Dyskin, A.: Mode I fractures with distributed bridges. Scaling and monitoring, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9365, https://doi.org/10.5194/egusphere-egu26-9365, 2026.

EGU26-16230 | ECS | Posters on site | NP7.1

Nonlinear wave group interaction in the long time evolution of wave trains 

Shuya Xie, Aifeng Tao, Jun Fan, Jinhai Zheng, and Chao Wu

The long time evolution of wave trains involves various nonlinear stages, with significant differences in the wave group shape at each stage. To further investigate the characteristics of nonlinear wave group interaction during the long time evolution of wave trains, the High-Order Spectral method and wavelet transform analysis are employed, and a novel spatial wave group identification method suitable for long time evolution process is introduced. Then the wave groups in the evolution process are classified into four types based on the wave group length. The results show that during the stage of modulation instability, all wave groups are of Type I, which is a result of modulation instability. In this stage, all wave groups propagate at the same velocity without any energy exchange between them, maintaining independent evolution. The appearance of the other three types of wave groups indicates the presence of nonlinear wave group interaction. Under the dominance of nonlinear wave group interaction, the number and length of wave groups no longer remain constant, with significant changes observed in their characteristic parameters. Additionally, the propagation velocities of the wave groups evolve continuously. When two wave groups with different velocities merge, the resulting group accelerates rather than decelerates. In the subsequent evolution, the participating wave groups begin to separate again, with the wave group that was initially trailing overtaking the one that was leading, and their velocities eventually approaching. It is worth noting that the different types of wave groups are the result of nonlinear interactions and also serve as the fundamental units for the subsequent nonlinear interaction processes.

How to cite: Xie, S., Tao, A., Fan, J., Zheng, J., and Wu, C.: Nonlinear wave group interaction in the long time evolution of wave trains, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16230, https://doi.org/10.5194/egusphere-egu26-16230, 2026.

EGU26-21671 | ECS | Posters on site | NP7.1

Influence of Thermal Effects and Material Disorder on Fracture Propagation 

Djamila Kebci

Crack propagation in heterogeneous materials is strongly influenced by the combined effects of temperature, microstructural disorder, and dissipation mechanisms, particularly in subcritical fracture regimes. Recent experiments performed on pressure-sensitive adhesive (PSA) tapes by S.Santucci et al at the École Normale Supérieure de Lyon (France) have revealed complex slow fracture dynamics, including intermittent and thermally activated propagation regimes under quasi-static loading conditions.

While these studies provide a detailed experimental characterization of adhesive peeling and fracture processes, the present work focuses on a theoretical investigation aimed at interpreting the underlying physical mechanisms observed experimentally. Within the framework of linear elastic fracture mechanics, we develop a model describing the time-dependent crack propagation kinetics by accounting for thermally activated processes and material disorder, in connection with energy-based approaches of the Griffith type. The model relates the elastic energy release rate and the stress intensity factor to the crack propagation velocity and allows us to analyze the influence of temperature on the transition from slow crack growth to unstable fracture. The results highlight the key role of thermal fluctuations in subcritical fracture processes and provide a consistent theoretical framework for interpreting experimental observations in adhesive materials.

How to cite: Kebci, D.: Influence of Thermal Effects and Material Disorder on Fracture Propagation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21671, https://doi.org/10.5194/egusphere-egu26-21671, 2026.

EGU26-1670 | ECS | Posters on site | AS1.22

Modelling climate change in the MLT with a gravity-wave permitting setup of UA-ICON 

Hannes Pankrath, Markus Kunze, Christoph Zülicke, Yanmichel Morfa Avalos, Nicholas Pedatella, and Claudia C. Stephan

The anthropogenic emission of carbon dioxide has been attributed as the main driver of global warming. However, its radiative properties also cause the middle atmosphere to cool and contract. This cooling, as well as associated changes in large-scale circulation patterns of the troposphere and stratosphere, result in trends in the mesosphere and lower thermosphere (MLT) region. We conducted a whole-atmosphere simulation employing the ICOsahedral Non-hydrostatic general circulation model with Upper Atmosphere extension (UA-ICON) in the configuration with the numerical weather prediction (NWP) physics package. As gravity waves are the main driver of the dynamics in the MLT and thus critically influence its thermal structure, we chose a horizontal resolution of 20 km to model a large portion of the gravity wave spectrum explicitly. A realistic large-scale circulation up to 50 km is ensured by constraining the dynamics of the troposphere and stratosphere to the ECMWF Reanalysis v5 (ERA5) dataset.
From the simulation, we derive trends of the atmospheric mean circulation and temperature. Additionally, the run is analyzed within the Transformed Eulerian Mean (TEM) framework to derive trends related to gravity waves and wave-mean flow interaction. For validation, the results are compared with the Atmospheric General circulation model for the Upper Atmosphere Research-Data Assimilation System (JAGUAR-DAS) whole neutral atmosphere reanalysis dataset (JAWARA).

How to cite: Pankrath, H., Kunze, M., Zülicke, C., Avalos, Y. M., Pedatella, N., and Stephan, C. C.: Modelling climate change in the MLT with a gravity-wave permitting setup of UA-ICON, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1670, https://doi.org/10.5194/egusphere-egu26-1670, 2026.

EGU26-1843 | ECS | Posters on site | AS1.22

Revisiting Intrinsic Predictability of Wave-Convection Coupled Bands Over Southern China: Variable and Scale-Dependent Error Growth Characteristics 

Manshi Weng, Junhong Wei, Yu Du, Y. Qiang Sun, and Xubin Zhang

This talk will present our recent work of Weng et al. (2025, in manuscript). Intrinsic predictability of the weather defines the ultimate limit of our day-to-day weather forecasts. This study aims to investigate the variable- and scale-dependent intrinsic predictability of wave-convection coupled bands lasting nearly 10 hours near the south coast of China on 30 January 2018, by conducting perturbed and unperturbed convection-permitting simulations with 1-km horizontal grid spacing under varying initial moisture conditions. In particular, the predictability time scale of each selected forecast variable is quantified in the current study via the Loss Predictability Index (LPI), defined as the ratio of the forecast error (difference between perturbed and unperturbed) power spectrum to the reference (unperturbed) power spectrum at a given scale or within a range of scales. Spectral analysis reveals substantial differences in the reference power spectral slopes among variables, while their error growth behaviors consistently exhibit upscale features. The intrinsic predictability limit of the banded convection, measured by the difference total energy (DTE), is approximately 7 hours. Predictability varies with both scale and altitude: smaller scales (i.e., ~10 km) have shorter limits than larger scales (i.e., ~40 km), and the middle-level moist neutral stability layer is less predictable than the low-level ducting stable layer. In particular, for the moist neutral stability layer, different variables become more correlated under the coupling between gravity waves and moist convection, yielding more coherent predictability characteristics. In the dry experiment, predictability exceeds 12 hours with minimal error growth, regardless of the variable, scale, or altitude. Finally, the decomposition of the horizontal kinetic energy spectrum into divergent and rotational components (proxies for unbalanced and balanced components, respectively), demonstrates contrasting power spectra, intrinsic predictability limits, and their sensitivity to initial moist content, with the divergent component exhibiting longer predictability in the ducting stable layer at wavelengths <40 km. These findings highlight how vertical flow structure, moisture content, and distinct dynamical components jointly constrain the intrinsic predictability of mesoscale convective systems.

Reference:

Manshi Weng, J. Wei, Y. Du, Y. Q. Sun, and X. Zhang, 2025: Revisiting Intrinsic Predictability of Wave-Convection Coupled Bands Over Southern China: Variable and Scale-Dependent Error Growth, Journal of Geophysical Research: Atmospheres (Major Revision).

How to cite: Weng, M., Wei, J., Du, Y., Sun, Y. Q., and Zhang, X.: Revisiting Intrinsic Predictability of Wave-Convection Coupled Bands Over Southern China: Variable and Scale-Dependent Error Growth Characteristics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1843, https://doi.org/10.5194/egusphere-egu26-1843, 2026.

EGU26-3063 | ECS | Posters on site | AS1.22

Denoising Stratospheric Nadir Sounder Observations using a Machine Learning Technique for Gravity Wave Detection 

Adam Hayes, Corwin Wright, Neil Hindley, Lars Hoffmann, and Phoebe Noble

Satellite observations of the atmosphere are often extremely noisy due to both hardware limitations and the inherent complexity of retrieving and making measurements of the atmosphere. Gravity waves, which are low amplitude signals present in the atmosphere, are hard to resolve in this data due to their relatively low amplitude and small spatial extent. As a result, noise becomes a limiting factor when trying to identify and characterise them in real observed data.

Current methods to address this problem often lean upon smoothing approaches; however, such approaches suppress small scale signals and reduce measured amplitude and momentum fluxes significantly. This impedes the process in developing the next generation of models where these waves must be resolved accurately.

A novel supervised machine learning approach is introduced which is able to accurately remove small scale noise features from nadir observations of gravity waves. This model was trained on synthetic observations derived from high resolution DYAMOND model runs.  This is then applied to 22 years of NASA AIRS data and 12 years of MetOp IASI data and used to produce a new gravity wave climatology to better access small amplitude gravity waves.

How to cite: Hayes, A., Wright, C., Hindley, N., Hoffmann, L., and Noble, P.: Denoising Stratospheric Nadir Sounder Observations using a Machine Learning Technique for Gravity Wave Detection, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3063, https://doi.org/10.5194/egusphere-egu26-3063, 2026.

EGU26-4568 | ECS | Orals | AS1.22

Measuring tropospheric gravity waves over stratocumulus cloud decks  

Mathieu Ratynski, Brian Mapes, and Hanna Chaja

Tropospheric internal gravity waves, often originating from jets, fronts, or deep convection, leave subtle but discernible imprints on the vast stratocumulus decks that cover subtropical oceans. These waves represent a non-negligible, yet poorly quantified, interaction between the free atmosphere and the marine boundary layer. This presentation introduces a robust, twopass methodology using 2D continuous wavelet transforms (CWT) on geostationary satellite imagery (GOES-16) to objectively detect, track, and characterize these wave packets. The core of our framework is its ability to precisely separate the intrinsic wave propagation signal from the dominant, large-scale advective flow of the cloud field.

Our method quantifies the primary physical signature of these waves: the modulation of cloudtop brightness caused by vertical displacements at the boundary layer inversion. By tracking these propagating brightness patterns, our algorithm identifies individual wave packets as dynamically evolving objects and measures their physical properties, including wavelength, propagation speed, and direction. To validate the method, we generate synthetic satellite imagery by superimposing the signatures of hypothetical wave fields (with known properties such as wavelength, speed, and direction) onto realistic, advected cloud scenes. This process allows us to confirm the method's ability to faithfully retrieve the initial parameters and to characterize its measurement uncertainties.

We then apply this validated methodology to a real-world case study from 12 October 2023 over the Southeast Pacific. The analysis successfully isolates a coherent wave packet with a ~150 km wavelength and tracks its dynamic evolution.

Potential applications are numerous, including the construction of wave climatologies, the study of wave-cloud interactions, the analysis of their role in organizing shallow convection, and the assessment of their long-range predictability. The tool, made available as open-source software, is intended to facilitate a systematic exploration of these key, yet often hidden, components of the climate system.

How to cite: Ratynski, M., Mapes, B., and Chaja, H.: Measuring tropospheric gravity waves over stratocumulus cloud decks , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4568, https://doi.org/10.5194/egusphere-egu26-4568, 2026.

EGU26-6563 | ECS | Posters on site | AS1.22

Data-Driven Gravity Wave Source Parameterization Using Machine Learning 

Erfan Mahmoudi, Zuzana Prochazkova, Stamen Dolaptchiev, Anke Pohl, and Ulrich Achatz

Representing gravity wave (GW) sources accurately remains a major challenge for climate models. While parameterizations for orographic and convective gravity waves are well established, studies have shown that additional sources, including fronts, jet streams, and jet exit regions, also generate gravity wave activity. These sources driven by dynamics are often not clearly defined in current parameterization methods, which leads to biases in momentum deposition and large-scale circulation.
In this study, we propose a machine learning-based framework to model gravity wave sources in a unified and data-driven way. We use high-resolution ICON simulations to resolve gravity wave generation from a wide range of atmospheric processes. A reduced-order representation of the gravity wave action density spectrum serves as the target function. This allows for a compact yet meaningful description of gravity wave emission. Input features include resolved large-scale flow characteristics, subgrid-scale orographic properties, and convective indicators taken from the model fields.
We train supervised machine learning models to learn the nonlinear relationship between the atmospheric state and the resulting gravity wave emission. The resulting parameterization accounts for gravity wave generation related not only to orography and convection but also to dynamically driven sources such as frontogenesis and jet-related processes.

How to cite: Mahmoudi, E., Prochazkova, Z., Dolaptchiev, S., Pohl, A., and Achatz, U.: Data-Driven Gravity Wave Source Parameterization Using Machine Learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6563, https://doi.org/10.5194/egusphere-egu26-6563, 2026.

EGU26-7463 | ECS | Orals | AS1.22

Using an oceanic acoustic noise model to evaluate and constrain simulated atmospheric states 

Pierre Letournel, Constantino Listowski, Marc Bocquet, Alexis Le Pichon, and Alban Farchi

Among the different types of atmospheric waves, infrasound corresponds to low-frequency acoustic waves that can propagate over thousands of kilometers within atmospheric waveguides formed between the  surface and the middle-atmosphere (MA, 15-90 km) or the lower thermosphere (90-120 km). Infrasound is a technology used to monitor the atmosphere for the Comprehensive Nuclear-test Ban Treaty (CTBT). Infrasound stations of the International Monitoring System put in place to monitor compliance with CTBT continuously record infrasound waves, which can be seen as a tracer of the MA and lower thermosphere dynamics. At these altitudes, Numerical Weather Prediction (NWP) models are biased, notably due to the lack of observations to assimilate, especially for winds, or for instance due to an approximate representation of the impact of atmospheric gravity waves on the dynamics. We propose a method based on the observation of infrasound of oceanic origin, known as microbaroms, to evaluate and compare the performances of atmospheric models in the middle atmosphere. We present a complete processing chain that simulates microbarom arrivals at an infrasound station and that compares them to observations. It explicitly accounts for both the oceanic source emission mechanism and the atmospheric propagation. Beyond the atmospheric diagnostics enabled by this method, we have implemented our modeling of microbarom arrivals within a variational data assimilation (DA) framework to constrain wind and temperature atmospheric fields in the MA. As proof-of-concept, first DA synthetic experiments were conducted in simplified atmospheric configurations to demonstrate the added value of infrasound observations in constraining the MA dynamics.

How to cite: Letournel, P., Listowski, C., Bocquet, M., Le Pichon, A., and Farchi, A.: Using an oceanic acoustic noise model to evaluate and constrain simulated atmospheric states, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7463, https://doi.org/10.5194/egusphere-egu26-7463, 2026.

EGU26-7532 | ECS | Posters on site | AS1.22

Spatial Distribution of Internal Tides in the Deep Southwestern Atlantic Ocean 

Xuehang Zhou, Zhiyuan Gao, and Zhaohui Chen

Internal tides are internal gravity waves with tidal frequencies, generated by the interaction of barotropic tides with rough seafloor topography. The breaking of internal tides constitutes one of the fundamental mechanisms for sustaining mixing within the deep ocean. However, past lack of large-scale deep-ocean observations caused uncertainties in characterizing their properties and spatial distribution patterns. The Southwestern Atlantic, with complex and diverse seafloor topography, provides an ideal site for studying deep-ocean internal tides while Deep Argo floats with full-water-depth observation capabilities enable this research. Based on data collected by Deep Argo floats during parking phase, the characteristics and spatial distribution of internal tides at 3000-4000 m in the deep Southwestern Atlantic Ocean are investigated. The analysis quantifies significant amplitudes of internal tides in the deep ocean, revealing spatial patterns distinct from the upper ocean. While upper-ocean internal tides are primarily modulated by large-scale topography, deep-ocean internal tides are subject to small-scale seafloor topography. Consequently, deep-ocean internal tides are spatially locked to local topography features rather than following far-field propagation paths, with semidiurnal internal tides exhibiting higher amplitudes in the Mid-Atlantic Ridge region, whereas diurnal internal tides are intensified near 28°S. These findings provide essential observational support for unraveling complex dynamics driven by small-scale seafloor topography.

How to cite: Zhou, X., Gao, Z., and Chen, Z.: Spatial Distribution of Internal Tides in the Deep Southwestern Atlantic Ocean, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7532, https://doi.org/10.5194/egusphere-egu26-7532, 2026.

Tropical cyclones (TCs) are a source of atmospheric gravity waves, which contribute to mixing in  the upper troposphere and lower stratosphere. Here, we conducted a large ensemble simulation run of the Weather and Forecasting Research (WRF, V4.4.1) model, assessing the impact of 15 combinations of microphysics (MP), planetary boundary layer physics (PBL), and a cumulus scheme (CU) on the model's ability to simulate the physics of Typhoon Soudelor (2015) and this typhoon's generation of gravity waves. The simulation is performed using a moving nested domain at 3 km  horizontal resolution, with a 15 km exterior main domain. We use data from International Best Track Archive for Climate Stewardship to measure bias in track position and intensity of the typhoon, supported by the use of AIRS/Aqua satellite observations as a benchmark. Moving beyond traditional analyses, we also apply a kernel density estimator (KDE) approach to produce more comprehensive results. 

Our results indicate that, while track errors remain below 100 km for the first 42 hours of the run, the simulated storm intensity and speed varied significantly from observations. Notably, simulations incorporating cumulus parameterization generally yield wider track spreads, whereas microphysics produced higher storm intensities and a more accurate representation of deep convective clouds compared to WSM6, despite an overall tendency to overestimate storm strength. We then examined coupling between tropical cyclone dynamics and stratospheric wave generation by comparing simulated Outgoing Longwave Radiation (OLR) and vertical wind speeds against satellite and reanalysis data. KDEs of OLR suggests, that while the Goddard MP effectively captures deep convection, the addition of a Grell-3 CU parameterization tends to produce more extensive mid-to-high-level cloud cover but underestimates the deepest convective cores. In the stratosphere, vertical wind speed profiles indicate that the MYJ and Goddard combinations produce the strongest wave activity, especially during the chosen peak events. Although the simulations slightly overestimate background wind speeds near the tropopause compared to ERA5 reanalysis output, the overall wave morphology remains consistent with observations. These findings reinforce the conclusion that no single physics combination optimally captures all TC attributes, though Goddard MP and specific PBL schemes offer superior performance in representing the convective forcing essential for stratospheric gravity wave excitation.

How to cite: Lu, Y.-S., Wright, C. J., Wu, X., and Hoffmann, L.: Sensitivity Analysis of Gravity Wave Characteristics to Physical Parameterization Options in WRF Simulations : A Case Study of Typhoon Soudelor (2015), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9749, https://doi.org/10.5194/egusphere-egu26-9749, 2026.

EGU26-9936 | ECS | Posters on site | AS1.22

Using ICON to model from ground to thermosphere - a global perspective 

Tom Dörffel and Claudia Stephan

We present a new global, high-resolution (10 km) simulation of the atmosphere using the ICON modeling framework and extending the vertical domain from the surface to the mid-thermosphere up to 250 km. With this configuration, gravity waves (GWs) are explicitly resolved up to a horizontal wavelength of about 50 km, and we can study the generation and dissipation across atmospheric layers, providing an opportunity to investigate GW propagation into the mesosphere and lower thermosphere (MLT) and their interactions with large-scale tides. Particular emphasis is put on cascading gravity waves, whereby primary waves generate secondary and higher-order GWs, and on their role in coupling the lower and upper atmosphere.

The simulation captures the interaction of gravity waves and tides with dynamically active regions, including the polar vortex leading to a sudden stratospheric warming (SSW). Achieving global, whole-atmosphere simulations at this resolution poses significant numerical challenges, including maintaining a consistent energy budget and ensuring the stability of the forward-in-time integrator across a wide range of scales and densities. We discuss strategies employed to address these challenges and assess their implications for model fidelity.

This modeling capability represents a critical step toward realistic whole-atmosphere prediction and provides an essential tool for the design and interpretation of coordinated satellite observation campaigns targeting GW–tide interactions and vertical coupling processes.

How to cite: Dörffel, T. and Stephan, C.: Using ICON to model from ground to thermosphere - a global perspective, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9936, https://doi.org/10.5194/egusphere-egu26-9936, 2026.

EGU26-10233 | ECS | Posters on site | AS1.22

Simulation of Internal Waves within an ALE ocean model: numerical challenges and modelling 

Andreas Alexandris-Galanopoulos and George Papadakis

Internal Solitary Waves (ISWs) are among the most important physical processes in oceanic systems. Specifically, they play a significant role in vertical mixing, energy transfer across the continental shelf, sediment resuspension, nutrient redistribution, and the regulation of thermocline structure. Their breaking and subsequent turbulent dissipation contribute significantly to the global energy cascade. Additionally, ISWs remain challenging to study: they are strongly nonlinear, inherently nonhydrostatic, and often require three-dimensional, high-resolution modelling to capture steep fronts, overturning, and mixing. Consequently, accurate numerical simulation of ISWs is vital for improving our understanding of their mechanisms and impact on ocean circulation and climate-relevant processes. 

Since the mid-20th century, numerical models have become indispensable tools for analyzing and predicting oceanic systems and processes. As such, considerable research has focused on developing discretization methods that faithfully simulate physical phenomena while minimizing numerical artifacts. Such frequent artifact is the Spurious Diapycnal Mixing (SDM), in which, due to numerical diffusion, the vertical advection scheme introduces mixing across the density layers, thus severely altering the stratification. Due to this, various methods to track and remedy SDM have been proposed [1]. 

SLS is a numerical ocean model introduced by A. Alexandris and co-authors in [2]. It uses a hybrid Finite Volume / Finite Element spatial discretization and treats the full pressure field through a Pressure Poisson equation. Thus, SLS is inherently a nonhydrostatic ocean model and can faithfully simulate dispersive phenomena, such as solitons. The main novelty of SLS is its Arbitrary Lagrangian Eulerian (ALE) scheme that suitably defines the vertical grid motion. 

Since the seminal paper, the ALE scheme of SLS was further improved through extensive numerical modelling and simulation of ISWs. To facilitate this, an optimization process was designed with the goal of reducing SDM. The optimality is expressed through a variational principle that defines the ALE grid motion through an elliptic equation. The mathematical derivation/ analysis of the scheme and its impact on SDM is organized in the preprint [3], which is submitted to Ocean Modelling and is under review. This also includes extensive simulations of ISWs including breaking and overturning on a sloping beach. 

In the present work, further experiences of simulating ISWs with SLS are presented. This includes the application of the ALE method to more challenging 3D turbulent simulations, where the ability of SLS to control SDM is further tested. Additionally, the stability of the ALE scheme is investigated, alongside analysis of some spurious behaviors that are caused by the interplay of the Lagrangian and Eulerian mesh dynamics. 

 References:

[1] Fox-Kemper, Baylor, et al. "Challenges and prospects in ocean circulation models." Frontiers in Marine Science 6 (2019): 65. 

[2] Alexandris-Galanopoulos, Andreas, George Papadakis, and Kostas Belibassakis. "A semi-Lagrangian Splitting framework for the simulation of non-hydrostatic free-surface flows." Ocean Modelling 187 (2024): 102290. 

[3] Alexandris-Galanopoulos, Andreas, and George Papadakis. "An ALE approach to reduce spurious numerical mixing through variational minimizers: application to internal waves." arXiv preprint arXiv:2511.20092 (2025) 

How to cite: Alexandris-Galanopoulos, A. and Papadakis, G.: Simulation of Internal Waves within an ALE ocean model: numerical challenges and modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10233, https://doi.org/10.5194/egusphere-egu26-10233, 2026.

EGU26-10944 | ECS | Orals | AS1.22

Impact of gravity waves on ice-cloud microphysics in a global NWP model using online coupling 

Alena Kosareva, Stamen Dolaptchiev, Axel Seifert, Peter Spichtinger, and Ulrich Achatz

Gravity waves (GWs) are well known for their role in shaping large-scale dynamics of the atmosphere, but they also induce strong local variability in the vertical velocity, temperature, and other fields.  Such variability is often omitted when it comes to global effects due to averaging and resolution limitations. However, small-scale dynamics, such as gravity waves, have a crucial role in cirrus microphysics and life cycle. Ice clouds, on the other hand, can have a pronounced effect on the Earth’s radiation budget and global moisture distribution, making their accurate representation in climate and numerical weather prediction (NWP) models particularly important.

This work investigates the effects of gravity waves on cirrus cloud microphysics using the global ICON (Icosahedral Nonhydrostatic) model. A novel, self-consistent parameterization of GW-induced homogeneous ice nucleation developed by Dolaptchiev et al. (2023) is employed, and additional GW effects on depositional ice growth are considered. The local GW field is represented using the Multi-Scale Gravity Wave Model (MS-GWaM), which supports multiple GW source types and three-dimensional wave propagation, thereby enhancing the physical realism of the parameterized GW dynamics. The full coupling of GW forcing, along with feedback from the supplemented ice scheme into the overall microphysics and radiation schemes, has been implemented and assessed within the ICON model.

The results of the global test runs reveal significant GW impacts on ice formation mechanisms, leading to enhanced homogeneous nucleation in the upper troposphere–lower stratosphere (UTLS) compared to the baseline ICON configuration. Furthermore, GW-induced temperature fluctuations obtained from MS-GWaM and coupled online to depositional growth substantially increase ice growth efficiency. It results in larger ice mixing ratios in the mid-latitudes and subtropical regions. Further analyses are planned to assess the sensitivity of the coupled version to different MS-GWaM configurations, the role of lateral GW propagation, and the relative contributions of different gravity wave sources.

How to cite: Kosareva, A., Dolaptchiev, S., Seifert, A., Spichtinger, P., and Achatz, U.: Impact of gravity waves on ice-cloud microphysics in a global NWP model using online coupling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10944, https://doi.org/10.5194/egusphere-egu26-10944, 2026.

EGU26-13026 | Orals | AS1.22

EnKF and EM based parameter estimation of a convective gravity wave parameterization using Strateole 2 constant level balloon data 

Francois Lott, Pierre Tandeo, Manuel Pulido, and Deborah Bardet

An offline methodology is applied to estimate parameters of a subgrid-scale non-orographic gravity-wave scheme using observations from constant-level balloons. The approach integrates the Ensemble Kalman Filter (EnKF) with an iterative parameter estimation method based on the expectationmaximization (EM) algorithm. The meteorological fields required for the parameterization offline are taken from the ERA5 reanalysis, corresponding to the instantaneous meteorological conditions found underneath the Strateole-2 balloon observations made in the lower tropical stratosphere from November 2019 to February 2021 and October 2021 to January 2022. Compared to a direct approach that minimizes a cost function and uses Bayesian inference of parameters, our analysis demonstrates that the EnKF/EM method effectively characterizes the launching amplitudes and altitudes of the parameterized gravity waves and while quantifying their associated uncertainties. Furthermore, we illustrate how the method can help improving a scheme, specifically the results indicate that introducing a background wave activity renders the convective wave parameterization more realistic.

How to cite: Lott, F., Tandeo, P., Pulido, M., and Bardet, D.: EnKF and EM based parameter estimation of a convective gravity wave parameterization using Strateole 2 constant level balloon data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13026, https://doi.org/10.5194/egusphere-egu26-13026, 2026.

EGU26-13124 | ECS | Posters on site | AS1.22

2D transient parameterization of gravity waves generated above an isolated mountain range 

Felix Jochum, François Lott, and Ulrich Achatz

Most operational gravity-wave parameterizations use single-column and steady-state approximations, thus neglecting horizontal propagation and transience. Recent studies indicate that these simplifications can lead to inaccurate predictions. Orographic gravity waves, e.g., can propagate over substantial horizontal distances, leading to the deposition of momentum far from their sources. The neglect of this could be a cause of regional momentum-flux deficits in atmospheric models, e.g. downstream of the Andes. Moreover, the variability of low-level winds can make mountain-wave generation a highly transient process, challenging the legitimacy of the steady-state approximation. This motivates the development of more complex models.

  MS-GWaM is a Lagrangian gravity-wave parameterization that is based on a multi-scale WKB theory allowing for both transience and horizontal propagation. In a previous study (Jochum et al., 2025), it was used in simulations within the idealized atmospheric flow solver PincFlow to investigate its ability to correctly describe the interaction between orographic gravity waves and a large-scale flow. 2D flows over periodic monochromatic orographies were considered, using MS-GWaM either in its fully transient implementation or in a steady-state implementation that represents classic mountain-wave parameterizations. Comparisons of wave-resolving simulations (not using MS-GWaM) and coarse-resolution simulations (using MS-GWaM) showed that allowing for transience leads to a significantly more accurate forcing of the resolved mean flow. The present study supplements MS-GWaM (within PincFlow's successor PinCFlow.jl) with a new blocked-layer scheme and continues the investigation with the more realistic case of an isolated 2D mountain range, where the impact of upstream blocking and horizontal propagation increases substantially, resulting in a more complex wave-mean-flow interaction. The blocked-layer scheme uses a relatively simple approach to blocking that is consistent with MS-GWaM's spectral representation of the unresolved orography. Its two parameters are calibrated via Ensemble Kalman Inversion, using a wave-resolving simulation as reference. The results show that the inclusion of this scheme yields a slightly improved forcing of the mean flow.

References

Jochum, F., Chew, R., Lott, F., Voelker, G. S., Weinkaemmerer, J., and Achatz, U. (2025). The impact of transience in the interaction between orographic gravity waves and mean flow. Journal of the Atmospheric Sciences.

How to cite: Jochum, F., Lott, F., and Achatz, U.: 2D transient parameterization of gravity waves generated above an isolated mountain range, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13124, https://doi.org/10.5194/egusphere-egu26-13124, 2026.

EGU26-17239 | Posters on site | AS1.22

Dynamical effects of atmospheric gravity waves in the upper troposphere and stratosphere as revealed by a high-resolution reanalysis. 

Petr Šácha, Zuzana Procházková, and Radek Zajíček

Gravity waves (GWs) are ubiquitous in stably stratified background states of the atmosphere from the boundary layer to the thermosphere. As a mesoscale phenomenon with typical scales smaller than the model effective resolution, they need to be parameterized in climate models based on numerous underlying simplifications. However, our understanding of the GW climate impacts is based mainly on their parameterized effects and may be model dependent and with uncertain relation to the real atmosphere dynamics.

                  Based on the whole span of the ERA5 reanalysis, here I present a "quasi - observational" assessment of GW dynamical effects in the extratropical upper troposphere and stratosphere. Part of our results confirms the textbook knowledge and expectations regarding the gravity wave role in decelerating the jet streams. But, after a closer inspection of the data, we found also previously unreported interactions and dynamical effects connected with GWs in the vicinity of the subtropical jet that can change the way how we parameterize them.

How to cite: Šácha, P., Procházková, Z., and Zajíček, R.: Dynamical effects of atmospheric gravity waves in the upper troposphere and stratosphere as revealed by a high-resolution reanalysis., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17239, https://doi.org/10.5194/egusphere-egu26-17239, 2026.

EGU26-17588 | Orals | AS1.22

Lead-time independence of gravity-wave forecast skill in operational analysis and forecasts 

Corwin J Wright, Peter Berthelemy, Neil P Hindley, Inna Polichtchouk, and Lars Hoffmann

Atmospheric gravity waves (GWs) are a key driver of vertical energy and momentum transport in the atmosphere, with important implications for large-scale dynamics and chemistry. However, they remain difficult to predict in operational weather and climate models due to their small spatial scales relative to model resolution, and are typically not assimilated into numerical weather prediction (NWP) systems because of the large departures they introduce from model initial conditions.Here we use stratospheric temperature measurements from the Atmospheric Infrared Sounder (AIRS) and the Cross-track Infrared Sounder (CrIS) to evaluate how well archived operational analyses and forecasts from ECMWF’s Integrated Forecast System reproduce observed GW activity over Greenland, a major Northern Hemisphere source region for orographic GWs. The combined AIRS–CrIS sampling at high latitudes provides an unusually high measurement cadence, enabling assessment of forecast performance and time variability at relatively fine temporal resolution.Operational analyses and forecasts with lead times of up to 240 h are sampled at the AIRS and CrIS measurement footprints and regridded to a common resolution to allow consistent spectral analysis. A 2D+1 Stockwell Transform is applied to both synthetic and real observations to characterise GW amplitudes and spatial structure, producing directly comparable GW fields across forecast lead times.Using a Structure–Amplitude–Location (SAL) framework adapted from precipitation forecast verification, we quantify the evolution of GW forecast skill with lead time. We find that model performance exhibits only weak dependence on forecast range: across all lead times, the model systematically produces GWs with smaller horizontal scales and reduced amplitudes relative to observations, while errors in wave location increase only modestly with lead time. This behaviour is unexpected, as shorter lead times are associated with more accurate resolved winds, and would therefore be expected to yield more accurate GW generation. The results suggest that errors in simulated GW characteristics in operational forecasts are dominated by structural and representational limitations rather than by forecast wind errors alone.

How to cite: Wright, C. J., Berthelemy, P., Hindley, N. P., Polichtchouk, I., and Hoffmann, L.: Lead-time independence of gravity-wave forecast skill in operational analysis and forecasts, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17588, https://doi.org/10.5194/egusphere-egu26-17588, 2026.

EGU26-19243 | ECS | Orals | AS1.22

Scattering of internal gravity waves by inhomogeneities 

Michael Cox, Hossein Kafiabad, and Jacques Vanneste

Internal gravity waves are scattered by inhomogeneities, such as background currents and bottom topography. Scattering modifies the wave's length and direction of propagation and in doing so, redistributes energy across wavenumbers and frequencies. When inhomogeneities are large relative to the waves, scattering reduces to a spectral diffusion process. Prior work on spectral diffusion considers only current-induced scattering via Doppler shift of the wave frequency. We generalise the diffusion framework to account for all large-scale inhomogeneities. This includes current-induced effects other than Doppler shift, and entirely different mechanisms such as scattering on bottom topography. We support our results with ray tracing simulations and analytical solutions.

 

How to cite: Cox, M., Kafiabad, H., and Vanneste, J.: Scattering of internal gravity waves by inhomogeneities, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19243, https://doi.org/10.5194/egusphere-egu26-19243, 2026.

EGU26-19909 | Posters on site | AS1.22 | Highlight

The MATS satellite: Mission update and 3-D mesospheric temperatures 

Linda Megner, Lukas Krasauskas, Jörg Gumbel, Donal Murtagh, Nickolay Icvhenko, Björn Linder, Jacek Stegman, Ole Martin Christensen, Jonas Hedin, and Julia Hetmanek

The MATS (Mesospheric Airglow/Aerosol Tomography and Spectroscopy) mission is a Swedish satellite mission designed to study atmospheric gravity waves the mesopause region. MATS was launched in November 2022 and carries a limb-imaging instrument that observes the Earth’s atmosphere in the altitude range from approximately 70 to 110 km and a nadir camera. The primary observables are airglow emissions in the O₂ A-band and ultraviolet light scattered by noctilucent clouds.

The limb instrument is a telescope that continuously images the atmospheric limb in six spectral channels: four channels in the near-infrared targeting the airglow, and two ultraviolet channels dedicated to noctilucent cloud observations. By exploiting limb geometry and multi-view sampling along the orbit, MATS enables tomographic reconstruction of three-dimensional atmospheric structures. The airglow measurements yield a high–vertical-resolution 3-D temperature product, allowing characterization of individual gravity waves, while the ultraviolet observations enable reconstruction of the spatial distribution and characteristics of noctilucent clouds.

This presentation will focus on the newly completed 3-D mesospheric temperature data set derived from the MATS airglow measurements. We will describe the tomographic retrieval, the characteristics and coverage of the temperature product. If available, early validation results will be presented.

The presentation will also provide an update on the current status of the MATS mission, which after severe technical and regulatory challenges since 2023, is expected to resume operations in February 2026.

How to cite: Megner, L., Krasauskas, L., Gumbel, J., Murtagh, D., Icvhenko, N., Linder, B., Stegman, J., Christensen, O. M., Hedin, J., and Hetmanek, J.: The MATS satellite: Mission update and 3-D mesospheric temperatures, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19909, https://doi.org/10.5194/egusphere-egu26-19909, 2026.

EGU26-20157 | ECS | Orals | AS1.22

Evaluations of wave-wave interactions for the oceanic internal gravity wave field at very high grid resolution  

Pablo Sebastia Saez, Manita Chouksey, Carsten Eden, and Dirk Olbers

Internal gravity waves (IGWs) play a key role in ocean dynamics by interacting with mesoscale eddies, topography, and other waves, leading to wave breaking and mixing that influence small and large-scale circulations. Despite local variability, the IGW energy distribution exhibits a remarkably universal spectral shape, the Garrett-Munk (GM) spectrum, within which we study the scattering of IGWs via wave-wave interactions under the weak-interaction assumption.

We use the kinetic equation derived from a non-hydrostatic Boussinesq system with constant rotation and stratification. By developing Julia-native numerical codes, we evaluate the energy transfers for resonant and non-resonant interactions. Our results confirm that resonant triads dominate energy transfers, while non-resonant interactions are negligible in isotropic spectra but can contribute under anisotropic conditions. We show that the Boltzmann rates are small such that the weak-interaction assumption is satisfied. We find non-local interactions to be essential to understand the energy transfers within the IGW field, while local interactions are of minor importance. Parametric subharmonic instability drives a forward energy cascade in vertical wavenumber and an inverse cascade in frequency. Induced diffusion emerges as a primary energy transfer to small scales, and elastic scattering plays a similar but weaker role. We also find a new interaction mechanism, the third parametric generation, which provides a forward energy cascade in frequency and vertical wavenumber. We assess the convergence of the kinetic equation by introducing a cutoff in the IGW energy spectrum, or with a change in slope mimicking the transition to turbulence. Our 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., Chouksey, M., Eden, C., and Olbers, D.: Evaluations of wave-wave interactions for the oceanic internal gravity wave field at very high grid resolution , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20157, https://doi.org/10.5194/egusphere-egu26-20157, 2026.

EGU26-20398 | ECS | Posters on site | AS1.22

Role of mixed layer turbulence on the generation of  internal waves  

Swarnali Dhar, Kannabiran Seshasayanan, and Eric D'Asaro

Turbulence in the ocean mixed layer is a major source of internal gravity waves, yet the efficiency and pathways of this energy transfer remain less understood. We investigate how mixed-layer turbulence excites internal waves and drives the rapid decay of mixed-layer kinetic energy following strong forcing events. Using numerical simulations of a turbulent mixed layer overlying a stratified interior, we explicitly resolve the generation and propagation of internal waves. The non-hydrostatic model shows that surface wave-generated turbulence in the mixed layer radiates high-frequency internal waves near the buoyancy frequency, exporting ~13% of the mixed-layer energy in 20 hours. A hydrostatic model shows that near-inertial baroclinic modes, especially mode 2, redistribute this energy vertically over 2–10 days. These mechanisms provide a fast, localized pathway for upper‑ocean mixing. Normal-mode and spectral analyses link this turbulent radiation to low-baroclinic modes, near-inertial adjustment, and anisotropic wave emission in the presence of a background flow. Together, these results provide compact scaling relations that connect observable mixed-layer properties and turbulence intensity to internal-wave energy fluxes, enabling realistic parameterizations of mixed–layer–to–interior energy transfer in ocean and climate models.

How to cite: Dhar, S., Seshasayanan, K., and D'Asaro, E.: Role of mixed layer turbulence on the generation of  internal waves , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20398, https://doi.org/10.5194/egusphere-egu26-20398, 2026.

Internal and inertial waves play a substantial role in ocean dynamics. They can transport a considerable amount of kinetic energy over long distances, and their amplitude in the abyssal ocean can reach gigantic vertical scales of several hundreds of meters. At the same time, packets of internal and inertial waves conserve a fixed angle with respect to gravity or the rotation axis upon reflection, which makes both their linear and nonlinear dynamics rather peculiar. Most hydrodynamical systems in closed domains can be described in terms of modes. In this framework, one usually assumes eigenfunctions satisfying the boundary conditions, for example Fourier standing modes in rectangular domains. These modes oscillate in time at every point in space but do not propagate in a specific spatial direction. Internal and inertial waves constitute a remarkable exception to this approach. It has been shown that, in a general geometry, wave beams of travelling waves converge toward a limiting path, known as a wave attractor, while global modes form a set of zero measure. Rectangular tanks aligned with gravity and/or rotation, actually represent an exceptional but very important case. Our work focuses on two aspects of internal waves in this context: first, the influence of the aspect ratio on the transition to turbulence and mixing for structurally stable wave attractors; second, the interplay between wave-attractor regimes and modal structures in the vicinity of rectangular geometries. Surprisingly, a conventional rectangular geometry may exhibit much more complex and strongly multistable regimes than those observed for simple wave attractors. We demonstrate competition between different triadic instability pairs, leading to multistability and a nearly uniform picket-fence spectrum, which is markedly different from the spectrum resulting from cascades of triadic instabilities driven by large-aspect-ratio wave attractors.

How to cite: Sibgatullin, I.: Aspect ratio effects, multistability and quantisation in wave attractors., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21268, https://doi.org/10.5194/egusphere-egu26-21268, 2026.

EGU26-21659 | Orals | AS1.22

Three-dimensional internal tide generation over isolated seamounts in a rotating ocean 

Nicolas Grisouard, Cécile Le Dizes, Olivier Thual, and Matthieu Mercier

Internal tides may cause a significant fraction of the diapycnal mixing required to maintain the meridional overturning circulation. Accurately understanding their generation in order to better represent it in global circulation models is therefore a critical step in improving climate science. To that effect, we introduce a boundary element method to solve the three-dimensional problem of internal tide generation over arbitrary isolated seamounts in a uniformly stratified finite-depth fluid with background rotation, without assumptions on the size or slope of the topography. We apply the model to the generation of internal tides by a unidirectional barotropic tide interacting with an axisymmetric Gaussian seamount. We qualitatively recover previously-derived two-dimensional results, including the documentation of topographies with weak energy conversion rates. Furthermore, our results reveal the previously underestimated influence of the Coriolis frequency on the wavefield and on the spatial distribution of radiated energy flux. Due to Coriolis effects, the energy fluxes are shifted slightly counter-clockwise in the northern hemisphere. We explain how this shift increases with the magnitude of the Coriolis frequency and the topographic features and why such effects are absent in models based on the weak topography assumption. Finally, we validate and discuss these semi-analytical results with the help of Large Eddy Simulations.

How to cite: Grisouard, N., Le Dizes, C., Thual, O., and Mercier, M.: Three-dimensional internal tide generation over isolated seamounts in a rotating ocean, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21659, https://doi.org/10.5194/egusphere-egu26-21659, 2026.

EGU26-1676 | ECS | Orals | OS1.2

Atmospheric and Climate Drivers of Extreme Swells Along the Peruvian Coast 

Gonzalo Agurto Barragan, Soledad Collazo, and Ricardo García-Herrera

Extreme swell events along the Peruvian coast pose recurrent risks to coastal communities, infrastructure, and maritime activities. These events originate far offshore, with their sources varying seasonally: during the austral winter they primarily develop in the South Pacific, while in summer they are typically generated in the western North Pacific. This study investigates the atmospheric circulation patterns associated with extreme wave events along the Peruvian coast generated in both hemispheres, with particular emphasis on the characteristics of the upper-level jet. Furthermore, the potential influence of climate change on the intensity of these events is assessed using an analogue-based methodology.

Events classified by the Peruvian Directorate of Hydrography and Navigation as very strong were selected for those originating in the Southern Hemisphere (SH), whereas strong events were selected for those originating in the Northern Hemisphere (NH). This difference is because events originating further away experience greater dissipation and therefore tend to be weaker. Using ERA5 reanalysis data, a composite analysis of atmospheric circulation revealed characteristic patterns in each hemisphere. SH events were associated with a dipolar cyclonic–anticyclonic pattern, producing strong pressure gradients, intense southwesterly surface winds, and an almost barotropic vertical structure. In contrast, events originating in the western North Pacific were linked to a deep cyclonic system, also exhibiting a barotropic structure. Complementing these results, analysis of the upper-level jet across multiple parameters indicates a more intense and latitudinally confined jet, generally exhibiting a positive tilt in both hemispheres. However, a key hemispheric difference emerges: in the SH, these features correspond to the polar front jet, whereas in the NH they reflect a strengthening of the subtropical jet.

Finally, to assess the anthropogenic influence on 10-m wind intensity between past and present periods, a flow-analogue approach was applied. In the SH, atmospheric circulation similar to those observed during the events is associated with stronger winds in the recent period. This intensification appears to be partly driven by the positive trend in the Southern Annular Mode, linked to anthropogenic ozone depletion and greenhouse gas forcing. In contrast, for events originating in the NH, the anthropogenic signal is less evident due to the pronounced interannual and interdecadal variability of the North Pacific, resulting in analogue-based reconstructions that show wind intensification in some events and weakening in others. Overall, these results highlight the distinct atmospheric dynamics governing swell generation in each hemisphere and provide insights that may inform early-warning systems, coastal risk assessments, and long-term adaptation strategies for Peru.

Acknowledgments: This work was supported by the SAFETE project, which has received funding from the European Union’s Horizon 2020 research and innovation program under the Marie Skłodowska-Curie grant agreement No 847635 (UNA4CAREER).

How to cite: Agurto Barragan, G., Collazo, S., and García-Herrera, R.: Atmospheric and Climate Drivers of Extreme Swells Along the Peruvian Coast, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1676, https://doi.org/10.5194/egusphere-egu26-1676, 2026.

EGU26-2792 | ECS | Posters on site | OS1.2

Effect of wave reflection on submerged plane slopes on the evolution of extreme wave fields 

Saulo Mendes, Jie Zhang, and Michel Benoit

Describing intricate concurrent wave processes frequently proves challenging and unwieldy. Although the influence of reflection rates on the development of extreme nonlinear waves remains poorly understood, controversy has emerged over whether elevated reflection rates amplify nonlinearity in the upper tail of the wave height distribution. Aided by fully nonlinear simulations, we present a theoretical framework that isolates the effects of shoaling length, bottom slope magnitude, and reflection rates. Comparing the simulation results with the theory for steep and reflective slopes, it is noticed that the theoretical excess kurtosis stabilizes for steep slopes with a high reflection rate, and that the simulated kurtosis remains in the confidence interval of our new theory. We therefore conclude that the high reflection rate is the main reason for anomalous wave statistics becoming stable.

How to cite: Mendes, S., Zhang, J., and Benoit, M.: Effect of wave reflection on submerged plane slopes on the evolution of extreme wave fields, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2792, https://doi.org/10.5194/egusphere-egu26-2792, 2026.

EGU26-3198 | Orals | OS1.2

Langmuir turbulence in a depth-varying coastal channel: Insights from large eddy simulations 

Tobias Kukulka, Todd Thoman, and Peter Sullivan

This study investigates wave-driven Langmuir turbulence (LT) in an idealized, depth-varying coastal channel representative of an estuarine bay or tidal river. In the open ocean, LT is a key turbulent process in the surface boundary layer, controlling the transport and mixing of momentum and density. LT arises from wave-current interactions that generate wind-aligned vortices, often visible as surface windrows of aggregated buoyant material such as plankton, bubbles, oil, and microplastics. To examine how LT influences the wind-, tide-, and density-driven circulation in a coastal channel, we develop a turbulence-resolving large eddy simulation (LES) framework with terrain-following coordinates representing a deeper central channel flanked by shallower margins. LT is generated through the Craik-Leibovich (CL) vortex force, which incorporates Stokes drift from wind-driven surface gravity waves. The simulations show that LT substantially enhances turbulent mixing, reducing vertical stratification and shear. Faster tidal currents in the deeper channel differentially advect salt, producing tidally varying lateral salinity gradients. These gradients generate baroclinically driven lateral and vertical tidal currents, whose development is both accelerated and intensified by LT. Conversely, vertical stratification and vertical shear of lateral currents can inhibit LT. Additionally, lateral shear of along‑channel currents associated with the channel bathymetry produces channel‑wide pairs of vertical vorticity that are tilted by Stokes‑drift shear, forming strong and persistent lateral circulations. Overall, the results reveal complex two‑way interactions between LT and the mean circulation, demonstrating that LT significantly modifies both tidally resolved and tidally averaged channel dynamics.

How to cite: Kukulka, T., Thoman, T., and Sullivan, P.: Langmuir turbulence in a depth-varying coastal channel: Insights from large eddy simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3198, https://doi.org/10.5194/egusphere-egu26-3198, 2026.

Accurate prediction of surface waves under tropical cyclones requires realistic representation of storm-induced ocean currents, which can strongly modulate wave growth and propagation. This study synthesizes results from a coupled modeling investigation and an observational analysis using drifting buoys deployed in four Gulf of Mexico hurricanes: Ian (2022), Idalia (2023), Helene (2024), and Milton (2024). The modeling system consists of the WAVEWATCH III wave model coupled to the Modular Ocean Model 6. The ocean model uses a mixing scheme that explicitly includes wave-induced Langmuir turbulence enhancement, resulting in reduced surface Eulerian currents that are more consistent with observations. The surface current introduced in the wave model combines the Eulerian current and the enhancement of the dominant wave group velocity arising from nonlinear interactions with coexisting waves. Idealized experiments show that omitting surface currents leads to systematic overestimation of maximum significant wave height by up to ~9%, with similar sensitivity to the specification of the upper-ocean mixing scheme. In real storms, drifter-based validation confirms that neglecting storm-induced currents results in consistent overestimation of significant wave height and peak period, particularly in regions of strong currents. These current-induced reductions in wave energy occur primarily because dominant wave packets propagate more rapidly and spend less time under intense winds. The effect is strongest in deep water but remains substantial in intermediate depths (20–70 m), where most observations were collected. Together, these results provide compelling evidence that storm-driven currents frequently reduce wave heights and periods under tropical cyclones. Incorporating realistic surface‐current effects into operational models is therefore essential for improving wave forecasts in tropical cyclones and enhancing coastal hazard assessments.

How to cite: Ginis, I., Papandreou, A., and Hara, T.: Wave Reduction by Storm-Driven Ocean Currents in Tropical Cyclones: Coupled Modeling and Drifting Buoy Observations , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4294, https://doi.org/10.5194/egusphere-egu26-4294, 2026.

EGU26-4487 | ECS | Posters on site | OS1.2

Fully Coupled Interactions between Sea Ice and Waves in the Bohai Sea under Different Ice Conditions 

Shi Qiu, Karsten.A Lettmann, Ayumi Fujisaki-Manome, Jia Wang, and Xueen Chen

A wave-ice interaction coupled model that resolves both ice-induced wave attenuation and wave-induced ice breakage was implemented within the Finite-Volume Community Ocean Model (FVCOM) framework and applied to the Bohai Sea, one of the lowest-latitude seasonally ice-covered seas in the Northern Hemisphere. Multi-source observations were used to validate the simulated wave and sea ice variables. We investigate wave–ice interactions under different ice conditions (mild, normal and severe ice years) and assess coupling effects by comparing a fully coupled (two-way) configuration with an uncoupled configuration and a one-way coupled configuration that accounts only for ice-induced wave attenuation. The presence of sea ice reduces wave energy and alters wave propagation. In turn, wave-driven processes exert complex influences on sea ice, potentially mediated by wave–current interactions, and wave activity can enhance melting along the ice fringe, highlighting the importance of explicitly representing two-way wave–ice interactions for accurately simulating ice-cover dynamics in the Bohai Sea.

How to cite: Qiu, S., Lettmann, K. A., Fujisaki-Manome, A., Wang, J., and Chen, X.: Fully Coupled Interactions between Sea Ice and Waves in the Bohai Sea under Different Ice Conditions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4487, https://doi.org/10.5194/egusphere-egu26-4487, 2026.

EGU26-4780 | Orals | OS1.2

On the higher-order wave-induced drift in deep water 

Raphael Stuhlmeier

The drift associated with the motion of inviscid, irrotational water waves was first derived by Stokes in the mid 19th century, and is today called Stokes drift. In deep water this takes the form us=a2kωe2kz0, where a is the wave amplitude, k the wavenumber, ω the radian frequency and z0 the initial particle depth. This formally second-order quantity is derived from linear theory, and is implemented in a wide variety of wave models to calculate the motion of marine contaminants and other passive tracers.

Adhering to linear wave theory, superposition allows for the immediate generalisation of the Stokes drift from a single wave to a wave spectrum. However, once more than one Fourier mode is included in the lowest order solution, nonlinear effects occurring at second and third order - chief among them the appearance of bound modes - should be considered when calculating Stokes drift.

We introduce a new, analytical correction to the Stokes drift

us= ∑j aj2ωjkje2kjz0+∑ki>kjωiai2aj2(ki-kj)2ij)-1e2(ki-kj)z0

under assumptions of unidirectional waves and deep water for analytical simplicity - and test this using direct numerical integration of particle paths [1]. Velocity fields for numerical work up to third order are obtained from the reduced Hamiltonian formulation of the water-wave problem due to Zakharov [2], and allow for the inclusion or exclusion of bound harmonics, amplitude evolution and dispersion correction to distinguish among competing effects. In particular, on the typical scale of particle motion the amplitude evolution can be neglected, allowing us to use an algebraic expression for the velocity field in terms of the (initial) Fourier amplitude spectrum [1]. Such an approach has also been successfully employed for deterministic forecasts of the ocean surface [3].

To summarise: we show how higher order contributions to the Stokes drift have an effect throughout the water column. At the surface this is connected to the critical role of high frequencies in the Stokes drift, where dispersion corrections are most influential, as well as contributions from sum-harmonic terms. At greater depths difference harmonics can come to dominate the flow-field and therefore the Stokes drift, as previously demonstrated for wave groups. All of this points to a need to reconsider the common formulation stemming from linear wave theory.

References:

[1] R. Stuhlmeier, Wave-induced drift in third-order deep-water theory, arXiv:2507.15688 (2025).

[2] R. Stuhlmeier, An introduction to the Zakharov equation for modelling deep water waves, D. Henry (ed.) Nonlinear Dispersive Waves (Springer Lecture Notes in Mathematical Fluid Mechanics), Springer (2024), pp. 99-131.

[3] M. Galvagno, D. Eeltink, and R. Stuhlmeier, Spatial deterministic wave forecasting for nonlinear sea-states, Physics of Fluids, (2021) 33 102116

How to cite: Stuhlmeier, R.: On the higher-order wave-induced drift in deep water, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4780, https://doi.org/10.5194/egusphere-egu26-4780, 2026.

EGU26-6877 | ECS | Posters on site | OS1.2

Experimental setup and first measurements of wind-wave interaction from the LéXPLORE platform on Lake Geneva 

Bryan Kunz, Maura Brunetti, Alexander Babanin, and Jérôme Kasparian

The interaction between wind and water waves is a complex process at the interface of two turbulent fluids. In this context, lakes provide conditions of intermediate complexity between the open ocean and wave tank experiments, allowing the investigation of fetch-limited wave responses under both directional and turbulent wind regimes, and in the absence of swells.

We developed an experimental setup installed on the LéXPLORE research platform on Lake Geneva (Switzerland) [1] to record the spatial and temporal variations of the water surface elevation using a pair of stereo cameras, as well as in situ wind profiles obtained with ultrasonic anemometers. To reconstruct the surface elevation and generate local directional spectra, we employ the optimised WASS algorithm [2], which has already proven effective during oceanic expeditions. The motion of the platform is tracked using an inertial measurement unit, which also helps refine wind-speed estimates. Moreover, the wave data are compared with in situ measurements acquired by buoys.

The LéXPLORE platform is ideally located for our study, as it simplifies the physical analysis and interpretation of the measurements. It lies far enough from the coast to ignore boundary effects, in deep water where bathymetry influences on wave propagation can be neglected, and at long fetch (for south-westerly winds) where wind forcing is maximised.

We will present the experimental setup and preliminary results on the reconstruction of directional spectra under different wind regimes during an experimental campaign in Spring 2026. 

[1] Wüest et al., WIREs Water 8, e1544 (2021)

[2] Bergamasco et al., Computers and Geosciences 107, 28 (2017)

How to cite: Kunz, B., Brunetti, M., Babanin, A., and Kasparian, J.: Experimental setup and first measurements of wind-wave interaction from the LéXPLORE platform on Lake Geneva, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6877, https://doi.org/10.5194/egusphere-egu26-6877, 2026.

EGU26-7925 | Orals | OS1.2

Real-time open ocean wind waves from navigation radars for a truly global wind wave operational observing system 

Sergey Gulev, Elizaveta Ezhova, Tilinina Natalia, Alexander Gavrikov, Vitali Sharmar, Boris Trofimov, Sergey Bargman, Peter Koltermann, Vika Grigorieva, and Alexander Suslov

Global information about ocean wind waves is crucial for understanding their role in the climate system, validating model outputs, and assessing risks for shipping and marine structures. Recent advances in marine radar technologies have enabled accurate, high-resolution measurements of surface wind waves and their spectral characteristics. Making these measurements available in real-time opens a wide new range of products for many user communities. Here we introduce SeaVision, a ship-based monitoring system that, once integrated into a standard shipborne X-band radar, considerably improves real-time observational networks along major shipping routes. SeaVision automatically measures significant wave height, peak period and directional wave spectra at temporal resolutions down to seconds. First developed for research purposes in 2020, SeaVision passed an extensive period of validation using Spotter wave buoys and satellite data. Validation onboard research vessels was conducted for a wide range of latitudes, from the Arctic to Antarctica. SeaVision is fully operational, cost‑effective, and capable of transmitting wave parameters continuously via satellite. Further developments of SeaVision allow for retrieving near surface wind speed, surface currents and ice parameters with the same resolution. Extensive installations of SeaVision (as well as similar systems) onboard commercial and research vessels allow for establishing a near-global observational network (as a part of GCOS and GOOS) largely exceeding capabilities of the present VOS network which over the last few decades are experiencing a dramatic decline and is also regionally complementing satellite missions. SeaVision will enhance coverage of the so far inadequately sampled global oceans.

How to cite: Gulev, S., Ezhova, E., Natalia, T., Gavrikov, A., Sharmar, V., Trofimov, B., Bargman, S., Koltermann, P., Grigorieva, V., and Suslov, A.: Real-time open ocean wind waves from navigation radars for a truly global wind wave operational observing system, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7925, https://doi.org/10.5194/egusphere-egu26-7925, 2026.

EGU26-8446 | Orals | OS1.2

Modelling and monitoring waves in the nearshore region 

Johannes Gemmrich, Becky Brooks, and Peter Holtermann

The nearshore region provides the link between the land and the ocean. Waves play a crucial part in many nearshore processes including sediment transport, coastal erosion, dispersion of pollutants, rip currents, and many more. It is also the region where most people interact with the ocean. Nevertheless, the nearshore is not well presented in operational wave forecasts.

Here we test the merit of resolving the nearshore region in a regional WAVEWATCH III ® setup. We test this for two contrasting wave climates: the swell-dominated west coast of British Columbia with tidal ranges up to 4m, and the fetch-limited, non-tidal western Baltic Sea with storm surges reaching +-1.5m. Both models are on unstructured grids, and we test the feasibility of zoomed-in regions of very high grid resolution. The effect of currents and water level are evaluated as additional forcing fields.

The models are validated against in-situ wave buoy observations including an array that tracks the wave evolution along two 2km shoaling paths. Gradual wave height reductions of >25% per km are observed, but little change in the spectral shape or directional characteristics.

 These observations are challenging to replicate in the model. We find that the inclusion of currents and water level yield the strongest improvement on significant wave heights and directional spreading, whereas increased grid resolution is beneficial for resolving small-scale bathymetric features.

How to cite: Gemmrich, J., Brooks, B., and Holtermann, P.: Modelling and monitoring waves in the nearshore region, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8446, https://doi.org/10.5194/egusphere-egu26-8446, 2026.

EGU26-10831 | ECS | Posters on site | OS1.2

Detection of Microscale Breaking in Wind-Driven Waves using a Colour Imaging Slope Gauge (CISG)  

Julián Marcelo Morales Meabe, Martin Gade, Camille Tondu, and Marc Buckley

Wind-driven gravity–capillary waves play a key role in air–sea interactions and in small-scale energy dissipation across the surface microlayer (SML). Despite decades of studies, the transition from smooth gravity–capillary waves to intermittent microscale breaking under weak wind forcing is still not well understood. 
This study investigates gravity–capillary wave dynamics and micro-breaking in a 24 m long, 1 m wide wind–wave tank with a total height of 1.5 m and a mean water depth of 0.51 m. Measurements were performed using a newly developed Colour Imaging Slope Gauge (CISG), providing high-resolution spatio-temporal observations of surface slopes within a 33.2 cm × 26.8 cm field of view (FOV), at a spatial resolution of 0.024² cm² per pixel and a frame rate of 400 Hz. A total of 18 experiments were conducted over a range of low wind speeds (1.8 m s⁻¹– 4.0 m s⁻¹) with small increments. Wire-wave gauge measurements were used to support three-dimensional surface reconstructions. 
Spectral, wavelet, and band-pass filtering techniques were applied to isolate capillary-scale features associated with micro-breaking. Particular attention was given to surface curvature as a geometric indicator of micro-breaking. The wide FOV enables direct tracking of isolated events and reveals a clear increase in capillary activity and micro-breaking occurrence with increasing wind forcing. 
First results indicate a distinct transitional regime at wind speeds near 2.0 m s⁻¹, where the first clear capillary signatures associated with micro-breaking emerge in the frequency-wavenumber spectra. The CISG successfully captures the spatial onset of 
these micro-breaking induced capillaries with wavelengths between 0.4 cm and 3 cm. 
By applying wavelet and band-pass filtering, these features were isolated, allowing for the identification of the "birth" of micro-breaking induced capillaries within the FOV. 
This work establishes a methodological framework for detecting micro-breaking and provides new insights into the surface conditions governing small-scale dissipation processes in wind-driven wave systems.

How to cite: Morales Meabe, J. M., Gade, M., Tondu, C., and Buckley, M.: Detection of Microscale Breaking in Wind-Driven Waves using a Colour Imaging Slope Gauge (CISG) , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10831, https://doi.org/10.5194/egusphere-egu26-10831, 2026.

EGU26-12764 | Orals | OS1.2

Including dynamic ocean surface waves in NorESM climate simulations 

Alfatih Ali, Mats Bentsen, Øyvind Breivik, Ana Carrasco, Jens Boldingh Debernard, Thea Ellevold, Clio Michel, and Thomas Toniazzo

Results from a suite of simulations with a version of the Norwegian Earth-System Model which includes an ocean surface-waves (OSW) component, WW3, are presented.
OSW are forced by surface winds in the control integration and may be additionally coupled to atmosphere, ocean and sea-ice components through several parametrisations dependent on wave-supported stress, wave significant height, Stokes drift, and wave radiant stress.
Significant effects on the simulated model climatology are found for each of such additional couplings.
However, for the processes considered, the effects of two-way coupling between atmosphere and OSWs, or between sea-ice and OSWs, are highly dependent on the model background climatology -- and therefore also on model systematic biases.
By contrast, additional mixing caused by Langmuir turbulence systematically causes the ocean mixed layer to deepen, with a robust impact on sea-surface temperatures (SSTs), viz mid-latitude cooling in the summer hemisphere, and mid-latitude warming in the winter hemisphere.
Replacing the dynamic OSW model, WW3, with an analytical scheme predicated on a local equilibrium sea-state (Li et al., 2017) to drive Langmuir mixing gives similar results, with a slight exaggeration of the deepening especially in the tropics likely due to missing wind-wave misalignment in the analytical formulation.

How to cite: Ali, A., Bentsen, M., Breivik, Ø., Carrasco, A., Debernard, J. B., Ellevold, T., Michel, C., and Toniazzo, T.: Including dynamic ocean surface waves in NorESM climate simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12764, https://doi.org/10.5194/egusphere-egu26-12764, 2026.

EGU26-14205 | ECS | Orals | OS1.2

Laboratory study of turbulent momentum and energy fluxes above/below microscale breaking wind waves, and influence of surfactants 

Camille Tondu, Marc Buckley, Martin Gade, and Julián Marcelo Morales Meabe

Exchanges of momentum and energy across the sea surface microlayer (SML)  are controlled by turbulent dynamics within the first millimeters above/below the wavy water surface. Wind-generated waves, ubiquitous at the ocean surface, strongly influence turbulent processes in the air and water near the surface, especially as the waves grow and (microscale) break. Surface-active substances, commonly found in coastal waters, are known to dampen waves over a wide range of scales. However, the influence of these surfactants on the coupled air-water flow dynamics and associated fluxes remains unclear. Indeed, some of the phenomena involved take place at a sub-millimeter scale, which makes it challenging to investigate the complex mechanisms at stake.

A combination of two experimental techniques (PIV, particle image velocimetry, and LIF, Laser Induced Fluorescence) with a high resolution (33 µm/pixel for the PIV and 55 µm/pixel for the LIF) were used to determine flow motions on both sides of the SML. The complex set-up was installed at a fetch of 15.5m at the 24-m long, 1-m wide, 1-5m high wind wave tank of the University of Hamburg (Germany) which is specially designed for studies with surfactants (Oleyl Alcohol, OLA in this work). Here, we focus on conditions with a reference windspeed of 4.5m/s measured by an ultrasonic anemometer at 64 cm above the water surface.

The wide field of view (51cm) enables us to capture the evolution in time and space of turbulent shear stress above and below individual wind waves. As the waves move through the field of view, steepen and microbreak, high magnitude turbulent shear is produced in the airflow past the wave-crest and can sometimes spread over several wavelengths when intense air-flow separation events occur. A quadrant analysis shows that negative momentum flux (Q1 and Q3) events are usually encountered before wave-crests whereas positive momentum fluxes (Q2 and Q4) events are produced past them on average. In the water, positive turbulent shear stress mainly shows up below the windward side of the waves, while negative turbulent shear is present below their leeward sides. An estimation of the viscous and turbulent energy dissipation integrated over the first centimeter underneath the water surface shows that the production of bound capillary waves enhances the energy dissipation, which becomes more intense as the capillary train grows up.

When surfactants are present, a reduction of sweeps and ejections (Q2 and Q4) past the dampened wave crests is notable and can be associated with the reduced occurrence and intensity of air-flow separation events. In the water, the removal of most capillary waves leads to a reduction in energy dissipation, as well as in the (phase) averaged turbulent kinetic energy below crests.

How to cite: Tondu, C., Buckley, M., Gade, M., and Marcelo Morales Meabe, J.: Laboratory study of turbulent momentum and energy fluxes above/below microscale breaking wind waves, and influence of surfactants, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14205, https://doi.org/10.5194/egusphere-egu26-14205, 2026.

EGU26-14883 | ECS | Posters on site | OS1.2

Synoptic characterization of extreme wind-wave events in Chile 

Magdalena Vasquez, Rene Garreaud, and Catalina Aguirre

Storm surges are phenomena caused by wind conditions of greater magnitude than usual, whether local or remote. The ocean-atmosphere interaction is important in the development of these events, since wind is the main factor that increases wave heights, leading to an increase in their energetic potential. For this reason, the study focuses on characterizing the meteorological conditions that triggered swells categorized as M3, M4 and M5 of the Escala de Impactos de Marejadas developed by the MarejadasUV (MUV) of the University of Valparaíso in the northern, central and southern areas of the country.
Three representative points were selected on the coasts of Chile: in the north (-23°S,72°W), in the center (-32°S,75°W) and in the south (-44°S,78°S). Datasets were extracted every 3 [hrs] for significant wave height, mean period, mean direction and wave energy spectra modeled with WaveWatch III forced with surface wind and sea ice area fraction from the ERA5 reanalysis. With these data, thresholds related to 2, 5 and 10 years of return period were obtained to categorize the events into M3, M4 and M5, respectively, that occurred between May and October from 1979 to 2022, obtaining 29 cases in the north, 28 in the center and 21 in the south.
The northern area was characterized by more remote swell events (24) than local (5). The latter have a similar configuration where the south winds (more commonly known as Surazo) developed swells of the three categories, with different wind magnitude. The remote events were generated by low pressure (LP) formed at different points of the study area mainly located below the 40°S in deep water. In the center area, there were a greater number of local events (8), which in addition to being formed by south winds were also formed by LPs developed near the study point and the shore. This last configuration being similar for the remote events (20), but the distance which they were developed was greater. In the southern area, there were more local events (17) than remote events (4), mainly formed by a LP that were formed nearly the study point.
In conclusion, the categorization of these events depends on the wave climate. Most of the local events in the north and center were formed by winds from the south. The rest of the events are developed by LPs originated in different parts of the study area.

How to cite: Vasquez, M., Garreaud, R., and Aguirre, C.: Synoptic characterization of extreme wind-wave events in Chile, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14883, https://doi.org/10.5194/egusphere-egu26-14883, 2026.

We present a preliminary study on the one-way coupling between the spectral wave model Wavewatch III (WW3) and the hydrodynamic model SCHISM (Semi-implicit Cross-scale Hydroscience Integrated System Model) to investigate wave–current interactions in the Columbia River estuary (USA) and its adjacent coastal ocean. WW3 is implemented on an unstructured grid, enabling high-resolution representation of the spatially complex conditions at the estuary mouth and extending into the open ocean, and it is forced with time-varying currents and water levels from SCHISM simulations. Preliminary results are compared with buoy observations and satellite-derived sea surface heights from the Surface Water and Ocean Topography (SWOT) mission, exploring the potential of these data for model evaluation. The study combines model evaluation using satellite and buoy data with the coupling of wave and hydrodynamic models in an estuarine environment, while highlighting the relevance of unstructured grids for representing fine-scale coastal processes within a broader oceanic context.

How to cite: Fernández, L., Seaton, C., and Haller, M.: Wave–Hydrodynamic Modeling of the Columbia River Estuary Using One-Way Coupling Between SCHISM and WAVEWATCH III on Unstructured Grids, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15527, https://doi.org/10.5194/egusphere-egu26-15527, 2026.

EGU26-16778 | ECS | Posters on site | OS1.2

Observations of Locally Generated Wind Waves using a Novel Airborne Polarimeter 

Goksu Duvarci and Nathan Laxague

Short wind-wave growth is central to estimating sea-surface drag and air-sea momentum transfer, as it increases surface roughness and facilitates directional wave breaking. Therefore, field observations that resolve the full wind-sea scale are essential for parameterizing air-sea fluxes and validating numerical weather prediction models.

In these efforts, we developed a measurement system with a polarimetric camera integrated into a UAV platform, leveraging RTK-enabled aircraft positioning and an inertial measurement unit for high-precision georeferencing. With varying altitudes, we resolve ocean waves ranging from centimeters to decameters, extending the polarimetric camera’s capabilities to those of wave buoys.

Field measurements were conducted from May to July 2025 on the coast of Rye, New Hampshire, under various conditions, including gusty winds, limited/unlimited fetch, and misaligned wind-swell and current. The observations yield 3D directional wave spectra, resolving wavelengths from 20 m to 6 cm and frequencies from 0.3 to 5 Hz. The directional spreading, current shear, and bimodal peaks are plotted against the mean current direction and wind speed, which were measured by a nearby buoy. With these measurements we aim to explore the dynamics of locally generated surface waves by linking the gravity capillary scales to larger wind-sea.

How to cite: Duvarci, G. and Laxague, N.: Observations of Locally Generated Wind Waves using a Novel Airborne Polarimeter, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16778, https://doi.org/10.5194/egusphere-egu26-16778, 2026.

EGU26-19619 | Orals | OS1.2

Impact‑based extreme‑wave intensity scale for high‑resolution coastal forecasting 

Catalina Aguirre, Sebastian Correa, Mauricio Molina, and Sergio Bahamondez

Extreme wave events are recurring meteorological and oceanographic hazards that have a significant impact on coastal regions, leading to infrastructure damage, beach erosion, and adverse effects on fisheries and port operations, resulting in substantial economic losses in Chile. In recent decades, both the frequency and intensity of extreme wave events have increased, and this trend is projected to continue due to climate change, making Chile's extensive coastline particularly vulnerable. In this context, having access to accurate and high-resolution coastal wave forecasting is crucial for coastal users and stakeholders involved in assessing and managing the risks associated with extreme wave events. Here, we present a high-resolution coastal wave forecasting system, which is validated using in situ measurements in Valparaíso Bay. Additionally, an impact-based extreme wave intensity scale has been developed to improve risk communication, support the issuance of official early warnings, and enhance emergency response. A five-category scale, derived from a qualitative analysis of historical impacts on beaches and coastal infrastructure, is fully integrated into the forecasting system. Video cameras have been installed to provide real-time broadcasts of the coastline, facilitating continuous monitoring of wave conditions and their impacts during extreme wave events. Furthermore, the information is disseminated through a dedicated public website and various social media platforms to effectively communicate warnings and promote preventive actions. Key national public institutions responsible for issuing warnings and managing emergencies participate in the information flow, thereby strengthening risk governance and public decision-making, and increasing confidence in the reliability of the coastal wave intensity forecasts.

How to cite: Aguirre, C., Correa, S., Molina, M., and Bahamondez, S.: Impact‑based extreme‑wave intensity scale for high‑resolution coastal forecasting, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19619, https://doi.org/10.5194/egusphere-egu26-19619, 2026.

EGU26-21071 | Orals | OS1.2

Compressible water-wave evolution equations for coupled gravity–acoustic modelling of long ocean waves 

Usama Kadri, Matthew Hunt, Ali Abolali, Jiwan Kim, Rachid Omira, and Ricardo S. Ramalho

Semi-analytical studies have demonstrated that water compressibility, seabed elasticity, and gravitational potential modify tsunami phase speed and can explain systematic arrival-time deviations observed in farfield measurements [1]. However, operational and research tsunami models remain based on incompressible formulations, preventing explicit simulation of acoustic modes and limiting investigation of gravity–acoustic coupling in large-scale free-surface flows.

We present the derivation and numerical implementation of a compressible set of water-wave evolution equations compatible with the widely used finite-volume tsunami modelling frameworks. Starting from the compressible Euler equations, the formulation retains weak compressibility and acoustic propagation while preserving the long-wave structure required for basin scale simulations. Particular attention is given to the pressure closure, dispersion relation, and numerical consistency with existing solvers.

The equations are being implemented within an open-source solver and validated against analytical limits and controlled numerical benchmarks. Preliminary results demonstrate stable coexistence of surface-gravity and acoustic modes, recovery of expected dispersion behaviour, and improved consistency of wavefront propagation speed relative to incompressible formulations. Synthetic impulsive source experiments of landslides illustrate the generation and radiation of coupled hydroacoustic–surface wave fields and their sensitivity to compressibility effects.

The proposed framework provides a physically consistent pathway for extending dispersion based corrections into fully time-dependent numerical models, which enables systematic investigation of gravity–acoustic coupling, compressibility effects, and wave–acoustic energy partitioning in long-wave ocean dynamics. The formulation also establishes a foundation for coupling numerical wave physics with hydroacoustic observations in future integrated modelling studies.

Reference

[1] A. Abdolali, U. Kadri, & J. Kirby, 2019. Effect of Water Compressibility, Sea-floor Elasticity, and Field Gravitational Potential on Tsunami Phase Speed. Scientific Reports, 9 (1), 1-8. 

How to cite: Kadri, U., Hunt, M., Abolali, A., Kim, J., Omira, R., and Ramalho, R. S.: Compressible water-wave evolution equations for coupled gravity–acoustic modelling of long ocean waves, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21071, https://doi.org/10.5194/egusphere-egu26-21071, 2026.

EGU26-21442 | Posters on site | OS1.2

Data-Driven Study of the Probabilistic Characteristics of Wind Waves in Latvia 

Laura Grzonka, Kevin Parnell, and Agnieszka Herman

Wind waves are inherently irregular and random, making the goal of finding a fully deterministic description practically impossible. However, knowing their probabilistic properties is crucial for engineering applications and for understanding ocean dynamics. To deepen this understanding and build more efficient wind-wave models, machine-learning approaches are likely to become increasingly valuable.  Recent progress in physics-informed machine learning (PIML) has transformed fluid mechanics by combining data-driven approaches with physical fundamental equations, enabling more robust and generalizable models.

In our study, we apply PIML techniques to identify probabilistic characteristics of wind waves. Our research is based on learning probability distributions directly from data, which allows us to avoid restrictive assumptions or classical approximations.

We utilize field measurements collected in Skulte, Latvia, during August–September 2022. The dataset includes pressure time series and 3D velocity profiles, providing a detailed description of wave dynamics. Building upon existing PIML architectures, we developed a framework capable of inferring an accurate and efficient probabilistic model of wind waves. Preliminary results show promising agreement with theoretical expectations and previous studies.

The dataset was provided by Kevin Parnell and colleagues from Tallinn University of Technology (TalTech), together with the Latvian Institute of Aquatic Ecology. Our findings highlight the potential of PIML for improving probabilistic wave modelling and set the foundation for future applications in coastal engineering and environmental monitoring.

How to cite: Grzonka, L., Parnell, K., and Herman, A.: Data-Driven Study of the Probabilistic Characteristics of Wind Waves in Latvia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21442, https://doi.org/10.5194/egusphere-egu26-21442, 2026.

EGU26-21550 * | Posters on site | OS1.2 | Highlight

Wave foecast models: what is missing?  

Alexander Babanin

Since their inception in the 1990s, the third-generation spectral models, used both for the operational wave forecast and for research, reached significant advances in their performance. This success, however, depends on the criteria for this performance and on the aims of the model usage. In the presentation, we will discuss what is missing and what applications require attention, revision or further development of model physics.

We will argue that the main problems, as far as the traditional aim of spectral models is concerned – the wave forecast, is with predicting swell, wave-current interactions and directional spectra of wind-generated waves. Swell is poorly predicted in terms of the wave height, but arrival time is its particular problem - swell can be up to 20 hours early or late by comparison to its forecast. We will demonstrate that partially this can be connected to the issue of wave-current interactions.

The problem of directional wave spectra connects us to a new role of wave models – providing the air-sea fluxes into coupled models for large-scale environments such as Atmospheric Boundary Layer, including spray production, tropical cyclone intensity, for modelling the upper ocean, including ocean mixing, air-sea gras transfer, biogeochemistry, for marginal ice zone, among other application, for climate. In the presentation, we will discuss the new criteria for model performances and avenues of reaching the new aims for spectral models in these new applications.

How to cite: Babanin, A.: Wave foecast models: what is missing? , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21550, https://doi.org/10.5194/egusphere-egu26-21550, 2026.

A comprehensive analysis of direct wind stress estimation is performed from a field campaign measurements carried out in the Gulf of Mexico. Air-sea interaction spar buoys were deployed and operated at three locations in order to study ocean-atmosphere interactions under a variety of meteorological conditions. Variability of atmosphere and ocean conditions is a very important issue that provide us with the best analysis of the influence of wave direction in the relative direction of wind stress upon the mean wind direction. Results of relatively simple cases with only one wave system show a gradual direction change of wind stress very much associated with the relative wave direction with respect to wind, specially under low to moderate wind conditions. These type of conditions are always more frequent in the ocean generally. When the calculation of the wind stress is performed in a reference frame aligned with wave propagation direction, a clearer evidence of the wave coherent stress component is observed. Main results of this work are obtained in such a coordinate system aligned with the waves claiming the paramount importance of the wave-coherent stress. The effect of multiple wave systems in the wind stress is addressed taken considering special conditions when atmospheric fronts were present in the region. The ultimate goal is to provide a proper parametrization of the momentum transfer to be used in the next generation of numerical models.

How to cite: Ocampo-Torres, F. J.: The influence of waves in wind stress direction as from the analysis of buoy direct measurements., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22146, https://doi.org/10.5194/egusphere-egu26-22146, 2026.

Accurate forecasting of ocean and climate can provide actionable information for decision-making and ocean governance, which is essential for transferring ocean science to sustainable development. However, huge common biases of ocean, typhoon and climate models hinder our forecasting ability. The programme of “Ocean to climate Seamless Forecasting system (OSF), approved by the UN Ocean Decade in 2022, aims to provide a solution. This presentation will introduce the OSF Programme and what it has achieved.

With huge heat content, ocean controls the evolution of TC and climate. In this regard, ocean is the key to improve forecasting ability. A key breakthrough of OSF is quantifying the dominant role of surface waves in upper-ocean mixing and air-sea fluxes, processes previously omitted in large-scale models. By integrating wave-induced physics into models, OSF has achieved fundamental improvements, reducing summer sea surface temperature bias in ocean models by ~80%, decreasing typhoon intensity forecast error by ~40%, and cutting climate model SST bias by ~60%. OSF further translates science into actions through its global network, innovative low-cost buoy observations, and operational systems such as OCEANUS and COAST, delivering actionable forecasts and tools for disaster risk reduction, ecosystem protection, and coastal resilience.

How to cite: Wang, S. and Qiao, F.: Towards Seamless Ocean-Climate Forecasting: Surface Wave Dynamics and the UN Ocean Decade OSF Programme, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22826, https://doi.org/10.5194/egusphere-egu26-22826, 2026.

EGU26-22828 | Posters on site | OS1.2

Enhanced Air-Sea Heat Flux during Cold Air Events: Observations and Mechanism Analysis 

Siyuan Wu and Fangli Qiao

Air-sea heat flux intensifies during cold airs and other strong weather events. However, due to the lack of long-term observations during such cold air processes, the quantitative enhancement of air-sea heat flux and its underlying mechanisms remain poorly understood. To address this issue, based on a tower-based platform in the southern Bohai Sea, a high-frequency turbulence measurement system was implemented to conduct a two-year air-sea flux measurement, collecting air-sea heat flux data covering 20 cold air outbreak events. This study quantitatively analyzes and reveals the pronounced variations in air-sea sensible heat flux of SHF and latent heat flux of LHF during cold air events, as well as the distinct roles of wind speed, air-sea temperature difference and specific humidity difference. The enhancement of SHFand LHF is further quantified. Our results show that the significant increases in wind speed and air-sea temperature difference are the primary drivers of the enhanced heat flux. Although LHF exhibits higher magnitude than SHF during cold air processes, LHF is predominantly controlled by increased wind speed, whereas SHF is mainly influenced by both wind speed and the air-sea temperature difference, with its enhancement being substantially greater than that of LHF. Compared to calm weather conditions, SHF and LHF under cold air conditions increased by an average of 12.8 and 1.6 times, respectively, while the total heat flux increased by 2.6 times on average. The increasement of heat flux can exceed 10 times during cold waves, even can reach the magnitude comparable to that observed during tropical cyclones.

How to cite: Wu, S. and Qiao, F.: Enhanced Air-Sea Heat Flux during Cold Air Events: Observations and Mechanism Analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22828, https://doi.org/10.5194/egusphere-egu26-22828, 2026.

NP8 – Emergent Phenomena in the Geosciences

EGU26-511 | ECS | Orals | CL5.8

Satellite-based detection of agricultural flash droughts and their ecosystem impacts in southeastern South America 

Lumila Masaro, Miguel A. Lovino, M. Josefina Pierrestegui, Gabriela V. Müller, and Wouter Dorigo

Flash droughts are rapid-onset events that develop within weeks, imposing severe and often unexpected impacts on agriculture. Their monitoring remains challenging due to several factors, including the scarcity of root-zone soil moisture (RZSM) observations and the lack of methodological consensus. This study has two main objectives: (1) to evaluate the applicability of the European Space Agency Climate Change Initiative Combined Root-Zone Soil Moisture product (ESA CCI COM RZSM) for detecting agricultural flash droughts (AFDs) across southeastern South America (SESA), and (2) to assess how satellite-based indicators obtained from the Moderate Resolution Imaging Spectroradiometer (MODIS) capture their physical evolution and agricultural impacts.

We apply two complementary AFD detection frameworks to ESA CCI COM and ERA5 RZSM data for 1979–2022: a statistical percentile-based approach and a physically based formulation derived from the Soil Water Deficit Index (SWDI). The percentile method detects AFDs as rapid transitions from above-normal to below-normal soil moisture. The SWDI identifies events through shifts from near-optimal water availability to physiological stress based on soil hydraulic properties. To evaluate agricultural impacts, we analyze satellite-derived evapotranspiration (EVT) and vegetation indicators from MODIS for two representative events in central-eastern and northern SESA. Vegetation indicators include the Land Surface Water Index (LSWI), fraction of absorbed Photosynthetically Active Radiation (fPAR), and Gross Primary Productivity (GPP).

Our results suggest that AFD detection is strongly conditioned by both methodological framework and dataset characteristics. The percentile-based approach tends to overestimate AFD occurrence in persistently wet or dry regimes, where small fluctuations are amplified after percentile transformation. In contrast, the SWDI-based approach preserves regional hydroclimatic gradients and provides a physically consistent representation of plant water stress. Regarding the dataset, ESA CCI COM RZSM captures the main spatial patterns and seasonal cycles of soil moisture depicted by ERA5 across SESA. However, it exhibits smoother short-term variability, delayed drying, and lower absolute soil moisture than ERA5, which could be attributed to the empirical filtering used to propagate surface signals into deeper layers.

Satellite-derived indicators effectively capture the evolution of AFDs across SESA. Soil moisture depletion is followed by reductions in EVT as ecosystems transition from energy- to water-limited conditions. Vegetation indicators respond shortly thereafter: LSWI reveals declining canopy water content, fPAR shows reduced photosynthetic activity, and GPP reflects suppressed ecosystem productivity. The magnitude and spatial extent of these impacts depend on antecedent soil moisture and land-cover type, highlighting the importance of background conditions in modulating drought severity.

Overall, the results demonstrate that ESA CCI COM RZSM provides valuable information for regional AFD monitoring when its physical limitations are considered. The coherence among soil moisture, surface fluxes, and biological responses highlights the potential of satellite observations to track the onset, intensification, and agricultural consequences of AFDs. These results strengthen the use of multi-sensor satellite systems for operational early-warning applications and impact assessment across climate-sensitive agricultural regions such as SESA.

How to cite: Masaro, L., Lovino, M. A., Pierrestegui, M. J., Müller, G. V., and Dorigo, W.: Satellite-based detection of agricultural flash droughts and their ecosystem impacts in southeastern South America, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-511, https://doi.org/10.5194/egusphere-egu26-511, 2026.

EGU26-1232 | ECS | Orals | CL5.8

Evaluating Divergent Evapotranspiration Feedbacks to Warming Across Water- and Energy-Limited Regimes 

Marco Possega, Emanuele Di Carlo, Annalisa Cherchi, and Andrea Alessandri

Land–atmosphere coupling is a central driver of climate variability and extremes, yet Earth System Models (ESMs) struggle to capture the complex interplay between hydrology, vegetation, and surface energy fluxes. In particular, the evapotranspiration–temperature (ET–T) feedback—a key mechanism linking soil moisture, vegetation water use, and near-surface climate—is poorly constrained, limiting confidence in projections of heat extremes and ecosystem stress. Here, we first assess ET–T feedback across a suite of post-CMIP6 ESMs for the historical period (1980–2014) as compared with available GLEAM observations; thereafter the ET-T feedback is investigated in a set of future idealized warming scenarios spanning multiple global temperature targets. To identify the physical and ecohydrological regimes controlling feedback strength, we apply the Ecosystem Limitation Index (ELI), which distinguishes energy-limited from water-limited conditions. Our results reveal a strong negative ET–T feedback in energy-limited regions, where evapotranspiration efficiently cools the surface and stabilizes temperature. In contrast, the feedback reverses in water-limited and transitional regions: here, worsening soil-moisture deficits suppress evaporation and reduce evaporative cooling, thereby amplifying surface warming. Comparison with GLEAM observations highlights regions where models succeed and fail in capturing these feedbacks, particularly in semi-arid ecosystems where land–atmosphere coupling is strongest. Future warming scenarios indicate an expansion of water-limited regimes, weakening negative ET–T feedbacks and reducing the ability of land surface to buffer temperature variability. This shift implies an increased risk of persistent heat extremes, stronger land-surface amplification of warming, and eco-hydrological transitions in sensitive regions. The findings of this study suggest priorities for next-generation ESMs: better representation of soil moisture dynamics, vegetation water-use strategies, and hydrological constraints.  

How to cite: Possega, M., Di Carlo, E., Cherchi, A., and Alessandri, A.: Evaluating Divergent Evapotranspiration Feedbacks to Warming Across Water- and Energy-Limited Regimes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1232, https://doi.org/10.5194/egusphere-egu26-1232, 2026.

Air pollutants can penetrate deep into the lungs, enter the bloodstream, and trigger a cascade of cardiovascular diseases. Elevated pollutant levels in cities are often associated with heavy traffic and industrial emissions, highlighting the need for effective mitigation strategies. Street trees can reduce air pollution through dry deposition, whereby particles are captured by tree canopies in the absence of precipitation. However, city-level models typically assume uniform deposition rates and neglect location-specific variation in tree benefits. Here, we designed a social-ecological systems approach (SES) and revealed substantial spatial disparities in tree-derived air quality benefits within a city. We found that communities with lower urban canopy received fewer air quality benefits. To address these differences, priority tree planting sites were determined using a stepwise framework that takes into account both neighbourhood-level population exposure and social vulnerability. Our findings demonstrate the uneven distribution of urban ecosystem services, emphasizing the importance of integrating environmental justice into urban forestry planning and provide practical guidance on optimizing planting for reducing population exposure to air pollutants. 

How to cite: Cui, S. and Adams, M.: Unequal Canopies, Unequal Benefits: Environmental Justice Implications of Street Tree Air Pollution Mitigation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2092, https://doi.org/10.5194/egusphere-egu26-2092, 2026.

EGU26-2682 | ECS | Posters on site | CL5.8

Constraining Flash Drought Projections Through Land-Atmosphere Coupling 

Yumiao Wang and Yuan Xing

The increasing drought onset speed is driving a global transition toward more frequent flash droughts, presenting unprecedented challenges for drought management and adaptation. However, projected changes in future flash drought characteristics show considerable divergence among climate models. Here, using models from the Coupled Model Intercomparison Project Phase 6 (CMIP6), we demonstrate that models capable of capturing the land-atmosphere coupling gradient between dry and wet soil conditions tend to project more pronounced global transition from slow to flash droughts in the future. This emergent relationship provides a robust constraint for future projections based on observed land-atmosphere coupling characteristics. Our analysis suggests that the societal and environmental risks posed by future flash droughts could be more severe than previously projected. Given the widespread impacts of flash droughts, this study not only enhances our understanding of uncertainties in drought projections, but also holds promise for supporting socio-economic planning and adaptation strategies through constrained projection.

How to cite: Wang, Y. and Xing, Y.: Constraining Flash Drought Projections Through Land-Atmosphere Coupling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2682, https://doi.org/10.5194/egusphere-egu26-2682, 2026.

In 2024, an exceptionally severe abrupt drought-to-flood transition (ADFT) event occurred over Henan Province in central China, causing substantial economic losses due to its abruptness and limited early warning. Although intraseasonal oscillations (ISOs) can provide precursors for forecasting extremes, previous studies have primarily focused on floods or droughts in isolation, leaving the synergistic impacts of multiple ISO modes on drought-to-flood transitions poorly understood. Here we show that the 2024 ADFT event was jointly modulated by two ISO modes with opposite propagation directions. During the drought stage, Rossby wave train maintained a Ural blocking pattern and displaced the westerly jet southward. This circulation configuration suppressed precipitation while enhancing temperature and sensible heat, leading to persistent drought conditions. During the transition-to-flood stage, both the Rossby wave train and the Western Pacific Subtropical High (WPSH) oscillation acted in concert. The southeastward-propagating Rossby wave train disrupted the blocking, while the WPSH oscillation migrated northwestward. Their combined effects shifted the rain belt northward, strengthened southerly moisture transport, increased latent heating, and ultimately triggered the extreme flood. The synergy between these two ISO modes amplified the transition magnitude by 50%, suggesting that the ADFT event would have been largely suppressed in the absence of their concurrent influence. These results underscore critical role of ISO phase evolution and propagation in ADFT events, and suggest that they may serve as useful precursors for forecasting abrupt transitions.

How to cite: Zhou, S. and Yuan, X.: The impact of intraseasonal oscillations on the 2024 abrupt drought-to-flood transition over central China, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2684, https://doi.org/10.5194/egusphere-egu26-2684, 2026.

EGU26-3979 | Orals | CL5.8

Assessing Canopy and Roughness‑Sublayer Turbulence Representation in Noah‑MP over Forest and Grassland at Lindenberg (Germany) 

Kirsten Warrach-Sagi, Frank Beyrich, Cenlin He, and Ronnie Abolafia-Rosenzweig

Land–atmosphere exchange in tall canopies is strongly controlled by turbulence within and above the canopy and in the roughness sublayer (RSL), where classical Monin–Obukhov similarity theory (MOST) is known to be imperfect. Recent developments in the Noah‑MP land surface model (LSM) include a unified turbulence parameterization that aims to provide a consistent treatment of turbulence from within the canopy, through the RSL, to the surface layer (Abolafia‑Rosenzweig et al., 2021). While this scheme has been tested primarily under snow‑dominated conditions, its performance for non‑snow, multi‑canopy environments over long time periods remains largely unexplored.

Here, we evaluate the unified canopy–RSL turbulence parameterization in Noah‑MP (version 5.1.1) using multi‑year, multi‑level observations from the Lindenberg observatory of the German Meteorological Service (DWD). We focus on two contrasting sites: (i) Kehrigk, a tall evergreen needleleaf forest canopy where RSL effects are expected to be strong, and (ii) Falkenberg, a short grassland site that more closely conforms to MOST assumptions. Both sites provide continuous 30‑min data since 2005, including eddy‑covariance fluxes of sensible and latent heat, radiation components, soil heat flux at 5 cm depth, skin temperature, and multi‑level profiles of air temperature, humidity, and wind speed up to 30 m (forest) and 10 m (grassland). All forcing and flux data undergo standard DWD quality control procedures.

Noah‑MP is run offline at both sites with identical land and soil parameterizations, driven by observed meteorology. We compare a standard configuration (MOST‑based surface‑layer and canopy treatment) with the unified canopy–RSL turbulence configuration. Beyond standard flux evaluation, we will diagnose friction velocity, Monin–Obukhov length, bulk transfer coefficients for heat and moisture, and the vertical structure of wind and temperature in the surface and roughness sublayers. Model performance will be analysed as a function of season, canopy type, and atmospheric stability.

By linking detailed, long‑term observations to alternative turbulence representations in a widely used LSM, this study aims to clarify under which conditions enhanced canopy–RSL formulations improve land–atmosphere coupling in next‑generation Earth System Models.

How to cite: Warrach-Sagi, K., Beyrich, F., He, C., and Abolafia-Rosenzweig, R.: Assessing Canopy and Roughness‑Sublayer Turbulence Representation in Noah‑MP over Forest and Grassland at Lindenberg (Germany), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3979, https://doi.org/10.5194/egusphere-egu26-3979, 2026.

Terrestrial water storage (TWS) is a key variable in the water cycle, and accurate estimation of TWS is crucial for understanding hydrological processes and improving hydrological prediction. In this study, we develop an AI-based data assimilation method for GRACE TWS observations, aiming to integrate the advantages of satellite observations and land surface models. The assimilation adopts the ResUnet model combined with a self-supervised learning strategy. Specifically, the ResUnet model is used to extract large-scale variation information from GRACE TWS observations and high-resolution information from the land surface model. This assimilation system is applied to the NoahMP land surface model for long-term simulation, and the performance is compared with the nudging method. Results show that the AI-based assimilation method is more conducive to depicting fine-scale hydrological processes. Quantitative evaluation indicates that the assimilation effect of the proposed method is superior to that of the nudging. In addition, validation against in-situ observations confirms the rationality and reliability of the proposed method, as it can more accurately estimate terrestrial water storage and related hydrological variables. In the future, this AI-based assimilation method can be extended to the assimilation of more hydrological variables and multi-source observations, which is expected to further improve the estimation capability of land surface hydrological variables and provide more reliable data support for water resource management.

How to cite: Zhu, E. and Wang, Y.: An AI-Based GRACE Terrestrial Water Storage Data Assimilation Improves Hydrological Simulation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4437, https://doi.org/10.5194/egusphere-egu26-4437, 2026.

The rapid development of numerical weather prediction (NWP) models offers new opportunities for improving quantitative precipitation forecasting, while raising challenges in objectively integrating multi-model forecasts. This study presents recent advances in an operational multi-model integration precipitation forecasting method based on the generalized Three-Cornered Hat (TCH) theory.Seven NWP models routinely operated at the National Meteorological Center of the China Meteorological Administration are considered, including ECMWF, GERMAN, NCEP, GRAPES_3KM, BEIJING_MR, GUANGZHOU_MR, and SHANGHAI_MR. The method applies TCH theory to estimate the relative error characteristics of precipitation forecasts from different models. A Bayesian framework is then used to derive objective, model-dependent weighting coefficients, enabling short-range multi-model integration forecasts.The integration performance is evaluated using Threat Score (TS) metrics for 2025. Results show that the TCH-based integration consistently outperforms the single ECMWF model across all precipitation categories. The 24-hour heavy rainfall TS reaches 0.2357, a 48% improvement, while the TS for extreme rainfall events reaches 0.1354, a 141% improvement relative to ECMWF.The multi-model integration products have been operationally implemented at the National Meteorological Center, providing critical support during high-impact weather events, highlighting both recent advances and remaining challenges in operational multi-model precipitation forecasting.

How to cite: chen, S.: Multi-model Integration Precipitation Forecasting Based on TCH Theory: Recent Advances and Challenges, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6074, https://doi.org/10.5194/egusphere-egu26-6074, 2026.

Ecosystem water use efficiency (WUE), an indicator of the trade-off between carbon uptake and water loss, is widely used to assess ecosystem responses to climate change. However, large-scale studies of WUE typically assume a single, fixed lag or accumulation period of climatic drivers across regions. This static assumption neglects spatially heterogeneous temporal responses of WUE to climate, potentially biasing attribution analyses and reducing predictive skill. Here, we developed a pixel-level model to quantify the temporal effects of climatic drivers on WUE by explicitly accounting for no-effect, lagged, cumulative, and combined effects and allowing effect timescales to vary spatially. We found that more than 80% of pixels across China exhibited lagged and/or cumulative effects for each driver, with distinct temporal effect patterns among vegetation types and drivers. In herbaceous cover croplands, precipitation exhibited the shortest lag (0.31 ± 0.56 months) and the longest accumulation time (1.71 ± 0.96 months). Accounting for these spatially heterogeneous temporal effects increased the explanatory power of climatic drivers for WUE variation by 17.7% compared with models without temporal effects. We further showed that for most vegetation types, precipitation and air temperature were more strongly associated with temporal variation in WUE, whereas solar radiation contributed more to spatial variability. These findings indicate that location-specific temporal effects can modulate the climatic controls on WUE. Our framework is readily applicable beyond China and can support a shift toward dynamic climate responses in climate–ecosystem interaction modeling, thereby improving forecasts of ecosystem dynamics and informing climate-adaptive vegetation management.

How to cite: Jiao, X.: Widespread Time-Lagged and Cumulative Effects Modulate Climatic Controls on Ecosystem Water Use Efficiency , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6580, https://doi.org/10.5194/egusphere-egu26-6580, 2026.

Abstract:To address the challenge of simulating runoff in ungauged regions, a hybrid physical–data-driven framework was developed by coupling Soil and Water Assessment Tool (SWAT) with an LSTM–Transformer. SWAT-derived process variables were fused with meteorological forcing to form a physically informed feature set for the Transformer-enhanced LSTM. The framework was first calibrated at a gauged station and then transferred to ungauged basins to evaluate its spatial generalizability. At the gauged station, the SWAT–LSTM–Transformer achieved the highest accuracy among all tested models, yielding an NSE of 0.587 and an R² of 0.728 on the validation dataset. It also maintained a better balance between calibration fit and validation robustness than SWAT–LSTM, SWAT–RF, SWAT–SVM, and stand-alone SWAT. SHAP-based interpretation revealed stable and hydrologically coherent predictor dependencies: temperature, lateral flow, and evaporation emerged as dominant drivers of the model’s runoff simulations, whereas precipitation and soil moisture exerted shorter-term and event-focused influences. When transferred to ungauged stations in the same watershed, the model reproduced seasonal runoff variations and event-scale fluctuations with high accuracy, with NSE ranging from 0.80 to 0.94 and R² from 0.83 to 0.92. Under cross-watershed transfer, the model continued to capture the main temporal patterns, with NSE and R² ranging from 0.62 to 0.83 and 0.60 to 0.84, respectively, although performance declined during extreme events. Overall, the coupled SWAT–LSTM–Transformer framework provides a robust and transferable approach for daily runoff simulation in data-scarce watersheds.

Key words: SWAT; LSTM-Transformer; runoff simulation; ungauged watersheds

How to cite: Peng, Z., Li, Y., and Liu, D.: An interpretable daily runoff simulation method in data-scarce watersheds by coupling SWAT and LSTM-Transformer, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7092, https://doi.org/10.5194/egusphere-egu26-7092, 2026.

EGU26-7919 | ECS | Posters on site | CL5.8

A dynamic representation of wetlands for the ISBA land surface model 

Lucas Hardouin, Bertrand Decharme, Jeanne Colin, and Christine Delire

Wetlands play a critical role in terrestrial hydrology and land–atmosphere exchanges, yet they remain poorly represented in many land surface models. Most approaches rely on static wetland maps, preventing models from capturing hydrological variability and associated feedbacks. Here we introduce a new dynamic wetland scheme in the ISBA land surface model, combining explicit hydrological processes with an annually varying diagnostic of wetland extent.

Wetland extent is computed using a TOPMODEL-based approach that links grid-cell saturation deficit with sub-grid topographic indices, and includes a correction for soil organic content to better represent peat-rich areas. Hydrological properties of wetlands and sub-grid runoff redistribution allow water to accumulate and persist in saturated zones, influencing the overall grid-cell water budget.

Simulated wetland extent shows good spatial agreement with multiple satellite-derived wetland datasets across a range of climate zones. Hydrological evaluation against GRACE-based terrestrial water storage and observed river discharge indicates that dynamic wetlands exert a modest but physically consistent influence on ISBA hydrology: they adjust discharge timing and magnitude without degrading model skill, while increasing grid-cell water storage and associated evapotranspiration. However, regional patterns of simulated evapotranspiration reveal a strong sensitivity to the assumed wetland vegetation type, underscoring the need for improved vegetation representation.

In particular, the dynamic wetland extent opens new opportunities for simulating wetland biogeochemistry, including methane emissions, and for exploring the key role of soil oxygen availability in controlling greenhouse gas fluxes.

How to cite: Hardouin, L., Decharme, B., Colin, J., and Delire, C.: A dynamic representation of wetlands for the ISBA land surface model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7919, https://doi.org/10.5194/egusphere-egu26-7919, 2026.

EGU26-8456 | ECS | Posters on site | CL5.8

C4MIP Multi-Model Projections of Moisture Convergence and Extreme Precipitation Risks over East Asia 

Nayeon jeon, Rackhun Son, and Dasom Lee

As extreme precipitation events intensify under climate change, understanding changes in precipitation patterns over East Asia has become increasingly important. While most future projections have relied on CMIP6 models, the Coupled Climate Carbon Cycle Model Intercomparison Project (C4MIP) integrates terrestrial–oceanic carbon cycle feedback including nitrogen deposition and biogeochemical processes to enhance the reliability of climate projection. Despite these advancements, C4MIP has been underutilized in hydrological assessments for East Asia. In this study, we analyze precipitation patterns over East Asia during the historical period (1980–2014) using a C4MIP multi-model ensemble and evaluate model performance through comparison with reanalysis datasets. The C4MIP ensemble demonstrates improved skill in capturing seasonal and interannual patterns of vertically integrated moisture flux convergence (VIMFC), particularly during periods of pronounced moisture convergence and divergence. Under the SSP5–8.5-bgc scenario, projection indicate intensified moisture convergence and increased risks of extreme precipitation over southeastern China and North Korea. These findings provide a diagnostic evaluation of C4MIP's hydrological performance and offer valuable insights for future regional climate projections and adaptation strategies.

 

This work was funded by the Korea Meteorological Administration Research and Development Program under Grant RS-2024-00404042 and the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (RS-2024-00343921).

How to cite: jeon, N., Son, R., and Lee, D.: C4MIP Multi-Model Projections of Moisture Convergence and Extreme Precipitation Risks over East Asia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8456, https://doi.org/10.5194/egusphere-egu26-8456, 2026.

EGU26-9964 | ECS | Posters on site | CL5.8

How do climate factors influence plant-based carbon sequestration in land surface model, and how does this change under global warming? 

He-Ming Xiao, Daniele Peano, Simone Mereu, and Antonio Trabucco

Gross primary production (GPP) is an important indicator of carbon uptake by ecosystems, and plants play a central role in ecosystem carbon sequestration. Understanding how plant-driven GPP fluctuates from year to year and which climate factors control these fluctuations is essential for assessing carbon sequestration. In addition, how carbon sequestration by these plants responds to a warming climate is still not well understood. The lack of high-resolution, well-networked, and long-term stable observations, together with mixed signals from land–atmosphere interactions, makes it difficult to identify and isolate the climate factors influencing plant-driven GPP from an observational perspective. In contrast, land surface models provide an alternative approach to addressing these limitations.

In this study, we conducted 5-km resolution simulations using a land surface model (Community Land Model Version 5, CLM 5, Lawrence et al., 2019) forced with high-resolution atmospheric datasets and updated land surface data covering the Italy and the western Mediterranean region. The high-resolution simulations allow for improved discrimination among different land types, such as urban areas and natural vegetation. We further articulated implementation of Corine land-cover data to better represent current land surface conditions and distribution of Plant Functional Types (PFT). Remarkable progress in the last years has increased representation of more and more complex processes incorporating, among others, plant and soil hydrological and carbon cycles, physiological and phenological processes, land surface heterogeneity and PFT parameterization in LSM. However, large limitations still remain due to uncertainties in representation of spatial and temporal dynamics of model parameters, sub-grid heterogeneity, and ultimately resolving optimal allocation and ecosystem functioning at small scales.  Mediterranean regions were selected as the focus of this study because, as climate change hotspot, they experience strong variability of ecosystem processes and dependencies to changing climate and to increasing severe drought-heatwaves compound events, making vegetation-based mitigation practices particularly urgent. 

We found that both temperature and precipitation play dominant roles in shaping interannual variations in GPP. Under cold or dry regimes, warmer temperatures and higher precipitation are beneficial for higher GPP. In contrast, under warm and wet regimes, further increases in temperature and precipitation are not beneficial for plant GPP production. We further used the model to identify suitable temperature and precipitation ranges for the growth of different plant types, and to examine how global warming is altering these ranges. Our analysis may provide implications for future afforestation practices, particularly in selecting forest types and specific climate/geographic zones that can achieve better carbon sequestration under a warming climate.

How to cite: Xiao, H.-M., Peano, D., Mereu, S., and Trabucco, A.: How do climate factors influence plant-based carbon sequestration in land surface model, and how does this change under global warming?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9964, https://doi.org/10.5194/egusphere-egu26-9964, 2026.

EGU26-11167 | Posters on site | CL5.8

An introduction to the EarthRes program 

Xing Yuan, Justin Sheffield, Ming Pan, Jonghun Kam, Xiaogang He, Joshua Roundy, Nathaniel Chaney, Niko Wanders, Linying Wang, Chenyuan Li, and Yi Hao

The High-Resolution Earth System Modeling, Analysis and Prediction for a Society Resilient to Hydrometeorological Hazards (EarthRes) is a program of the International Decade of Sciences for Sustainable Development (IDSSD), endorsed by UNESCO in 2025. EarthRes aims to build global societal resilience to hydrometeorological hazards through five pillars: (1) establishing cooperative observation networks; (2) advancing process-based understanding of Earth system dynamics; (3) enhancing prediction and early warning capabilities; (4) fostering indigenous and local knowledge and data sharing; and (5) strengthening capacity building among international partners.

This presentation will introduce the program's recent progress, including collaborative observations for understanding Earth system dynamics, the integration of a regional climate model with a coupled land surface-hydrology-ecology model that accounts for human activities (e.g., reservoir regulation, irrigation, urbanization), and the development of a forecasting framework. This framework connects the regional model with an AI model to predict droughts, floods, and compound events at synoptic to sub-seasonal scales.

Other activities under EarthRes will also be introduced, and future plans will be discussed. Through international collaboration and targeted capacity-building, EarthRes seeks to enhance sub-seasonal prediction and early warning capabilities, with particular benefits for vulnerable regions.

How to cite: Yuan, X., Sheffield, J., Pan, M., Kam, J., He, X., Roundy, J., Chaney, N., Wanders, N., Wang, L., Li, C., and Hao, Y.: An introduction to the EarthRes program, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11167, https://doi.org/10.5194/egusphere-egu26-11167, 2026.

EGU26-13594 | ECS | Posters on site | CL5.8

Classification and Attribution of Compound Flood Events  

Jinjie Zhao and Carlo De Michele

Floods are the most common natural hazards, and the compound effects of flood events pose severe challenges to flood protection. The lack of flood observation data makes it difficult to identify and analyze compound flood effects. Here, we employed a data-driven approach to reconstruct discharge in ungauged regions. We classified flood events from a compound perspective, quantified the contributions of different drivers, and compared the impacts of compound and non-compound flood events. Our results showed that pronounced compound effects were common in most flood events, with many compound flood events clustered in India and southeastern China. Compound events caused substantially greater impacts than non-compound events in Asia and North America.

How to cite: Zhao, J. and De Michele, C.: Classification and Attribution of Compound Flood Events , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13594, https://doi.org/10.5194/egusphere-egu26-13594, 2026.

EGU26-14172 | ECS | Posters on site | CL5.8

Benchmarking machine learning-based emulators and traditional methods to calibrate land model parameters for 124 global flux tower sites 

Ignacio Aguirre, Wouter Knoben, Nicolas Vasquez, and Martyn Clark

Accurately simulating latent and sensible heat fluxes is a long-standing open challenge in the land modeling community. The recent model intercomparison project PLUMBER 2 over 154 flux towers showed that simple 1-variable linear regression models can outperform process-based models in simulating latent and sensible heat. PLUMBER 2 simulations were run using default model parameters, leaving the potential performance gains from parameter estimation unquantified.

Identifying optimal parameters in land models has several challenges, including high computational cost and the need to identify parameters that can correctly reproduce temporal dynamics (i.e., good performance across different time epochs) and spatial patterns (i.e., good performance across many sites). To evaluate the ability of different calibration methods to handle these challenges, this study compared the performance of traditional and machine-learning emulator-based calibration methods against Long Short-Term Memory (LSTM) benchmarks, with single-objective experiments (latent heat or sensible heat calibrated individually) and multi-objective experiments (latent and sensible heat calibrated simultaneously). We also tested two ways to train emulators and LSTMs: either considering one site at a time or leveraging information from multiple sites and their attributes simultaneously.

Our results show that the calibrated simulations outperformed the default parameters and the simple benchmarks used in PLUMBER 2, demonstrating the potential to improve process-based models. Moreover, we observed that traditional calibration methods have a tendency to overfit: these traditional calibration methods can achieve high performance during calibration but are unable to achieve similar results during validation. The emulator-based methods achieve more consistent results across both calibration and validation time periods. Additionally, we found that parameter estimation methods that incorporate information from multiple sites simultaneously achieve better spatial consistency than methods that only learn from one site at a time. These results suggest that the performance gap between LSTM and process-based models can be significantly narrowed through calibration.

 

How to cite: Aguirre, I., Knoben, W., Vasquez, N., and Clark, M.: Benchmarking machine learning-based emulators and traditional methods to calibrate land model parameters for 124 global flux tower sites, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14172, https://doi.org/10.5194/egusphere-egu26-14172, 2026.

Land hydrology is a fundamental part of the global water cycle, and as such, of Earth’s climate system, including the biosphere. Yet, this basic component is still poorly represented in current models, partly because the structure of the land features scales much smaller than what those models can resolve, but also due to a lack of understanding of processes occurring below ground that are not readily at sight. Here we will examine from the perspective of what is important to the atmosphere from seasonal to centennial timescales, questions such as what groundwater and surface water do in shaping water availability and how vegetation and ecosystems adapt to it, ultimately modulating land-surface fluxes and climate. How relevant are these processes and what are we missing in current land-surface models? 

How to cite: Miguez-Macho, G. and Fan, Y.: Land hydrology, water availability for ecosystems and land surface models: what are we missing? , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15491, https://doi.org/10.5194/egusphere-egu26-15491, 2026.

Human interactions with the water cycle are increasingly recognised as critical drivers of land-climate feedbacks, yet they have long been under-represented in climate modelling.  With ongoing climate change, water management strategies and irrigation practices are becoming more important across many parts of the world. Since these activities can significantly alter surface energy and water fluxes, and thus local and regional climate, it is important to study these processes in more detail.

Although some Earth system models and regional climate models have started to incorporate irrigation routines, they still lack a representation of water availability from different sources and the competing demands of other sectors. To address this gap, we are developing the flexible water modelling tool C-CWatM that can be easily coupled with existing (regional) climate models. Based on the socio-hydrological model CWatM, it simulates river discharge, groundwater, reservoirs and lakes, as well as water demand and consumption from industry, households and agriculture.

In this contribution, we present initial results from coupled simulations using C-CWatM and the regional climate model REMO to study the impact of large-scale irrigation on regional climate conditions. The coupling is implemented via the OASIS3-MCT coupler, which manages synchronised data exchange and regridding of coupling fields. REMO provides the forcing fields required by C-CWatM and receives irrigation water amounts from C-CWatM, which are then applied within REMO's irrigation scheme. 

The development and coupling of C-CWatM allows climate models to realistically account for irrigation constraints, which is particularly important in water-scarce regions and under the increasing risk of droughts driven by climate change. Thus, our approach is an important step towards next-generation land surface modelling and promotes collaboration between hydrology and climate modelling communities to advance understanding of land-climate feedbacks and inform future adaptation strategies.

How to cite: Schmitt, A. and Greve, P.: Irrigation–climate feedbacks in coupled climate simulations: First results using an integrated hydrological modelling tool, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17003, https://doi.org/10.5194/egusphere-egu26-17003, 2026.

EGU26-17882 | ECS | Posters on site | CL5.8 | Highlight

Rapid Forecasting Method for Flood Process by Using on Physically Based Numerical and AI Model 

Xinxin Pan and Jingming Hou

With the acceleration of urbanization, complex underlying surfaces, pipe networks, river channels, and hydraulic facilities (gates, sluices, pumps) have significantly increased the number of computational grids and physical processes, making the computational efficiency of physical rainfall-runoff models insufficient to meet the timeliness requirements of emergency management for flood disasters. This necessitates further research on new technologies to enhance the computational efficiency of flood simulation and forecasting models. The development of AI technology provides new approaches for rapid flood disaster simulation and forecasting. This study proposes three innovative methods to address these challenges. First, GPU Accelerated Model for Surface Water Flow and Associated Transport. Second, AI Based Rapid Predicting Method for Flood Process. Third, Model Application for Dam Break Flood Simulation. 

How to cite: Pan, X. and Hou, J.: Rapid Forecasting Method for Flood Process by Using on Physically Based Numerical and AI Model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17882, https://doi.org/10.5194/egusphere-egu26-17882, 2026.

EGU26-18864 | ECS | Posters on site | CL5.8

Global amplification of water whiplash revealed by terrestrial water storage 

Yuheng Yang and Ruiying Zhao

Hydroclimate volatility, characterized by abrupt transitions between dry and wet extremes, poses a growing threat to global water security. Yet, current understanding of these transitions largely relies on meteorological metrics, which often fail to capture the full complexity of hydrological processes, land surface memory, and human water management. Here, we present a global assessment of water whiplash through the lens of terrestrial water storage (TWS). By integrating hydrological modeling with data-driven approaches, we reconstructed a comprehensive long-term TWS dataset to identify these events and account for delayed hydrological responses. Our results reveal a widespread intensification of global water whiplash in recent decades, with a substantial further increase projected under high-warming scenarios. Attribution analysis indicates that while climate change acts as the dominant driver of this amplification, human water management plays a critical role in spatially modulating these events, capable of either significantly mitigating or exacerbating local volatilities. We identify key hotspots of intensification in the tropics and high latitudes, encompassing extensive agricultural regions and major river basins. These findings establish TWS as a vital integrative indicator for monitoring abrupt hydrological transitions and underscore the urgent need for adaptive water management strategies to navigate an increasingly volatile hydroclimate.

How to cite: Yang, Y. and Zhao, R.: Global amplification of water whiplash revealed by terrestrial water storage, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18864, https://doi.org/10.5194/egusphere-egu26-18864, 2026.

EGU26-19214 | ECS | Orals | CL5.8

Introducing Groundwater Dynamics into the ECLand Land Surface Model: Implementation and Effects 

Vincenzo Senigalliesi, Andrea Alessandri, Stefan Kollet, and Simone Gelsinari

Land surface models still lack a realistic representation of groundwater, often relying on a free drainage condition at the bottom of the unsaturated soil column as in the current version of ECLand. This unrealistic assumption places the groundwater infinite depth below the surface, thus limiting the model’s ability to simulate realistic soil–vegetation-groundwater interaction.

To address this limitation, we implemented a Dirichlet boundary condition at the bottom of the unsaturated soil to enable a fully implicit numerical scheme for coupling with groundwater. First, we prescribed the water table depth (WTD) using global scale estimates to allow for the computation of realistic water fluxes between the unsaturated zone and the underlying aquifer. In a second step,  a dynamic WTD (hereafter the DYN configuration) was  developed by defining the water stored in the  unconfined aquifer, which evolves prognostically according to drainage (groundwater recharge) and subsurface runoff (groundwater discharge).

The effects of these developments were preliminarily evaluated through offline land-only simulations forced by station data from the PLUMBER2 project, which includes observational networks such as FLUXNET2015, La Thuile, and OzFlux. We validated the DYN configuration against the model setup with free-drainage conditions (CTRL). Our results show a systematic improvement in both latent and sensible heat fluxes, as quantified by the reductions in the error metrics  across most stations, with runoff scoring the best performances. 

The results of the global simulations largely corroborate and expand upon those of the station-based evaluation experiments conducted using PLUMBER2. The DYN configuration provides a more accurate representation of WTD, both spatially and temporally. This is evident in global climatological maps and independent observational datasets. Additionally, latent and sensible heat fluxes are consistently better represented in DYN than in CTRL, showing closer agreement with DOLCE and GLEAM products. Improvements are also evident in runoff simulations, with DYN exhibiting greater consistency with GLOFAS observations. Model performance was further evaluated against multiple observational datasets, such as GRACE/GRACE-FO to verify temporal variability in total water storage and to assess long-term mean conditions.

This work demonstrates that incorporating  groundwater dynamics significantly improves the realism of land-surface processes, particularly in the representation of the flux exchange of water and energy with other components. These results provide a foundation for the enhancement of the representation of land-climate interactions and hydroclimatological behaviour in next generation of reanalysis and climate predictions.

How to cite: Senigalliesi, V., Alessandri, A., Kollet, S., and Gelsinari, S.: Introducing Groundwater Dynamics into the ECLand Land Surface Model: Implementation and Effects, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19214, https://doi.org/10.5194/egusphere-egu26-19214, 2026.

EGU26-19820 | Posters on site | CL5.8

 Surface Soil Moisture–Vegetation Feedbacks in Water-Limited Regions across Land Surface Models 

Andrea Alessandri, Marco Possega, Annalisa Cherchi, Emanuele Di Carlo, Souhail Boussetta, Gianpaolo Balsamo, Constantin Ardilouze, Gildas Dayon, Franco Catalano, Simone Gelsinari, Christian Massari, and Fransje van Oorschot

Soil moisture plays a critical role in water-limited regions through its strong coupling and feedbacks with vegetation. However, state-of-the-art Land Surface Models (LSMs) used in reanalysis and near-term prediction systems still lack a realistic coupling of vegetation, limiting their ability to properly account for the fundamental role of vegetation in modulating the feedback with soil–moisture.
In this study, we incorporate Leaf Area Index (LAI) variability from observations - derived from the latest-generation satellite products provided by the Copernicus Land Monitoring Service - into three different LSMs. The models perform a coordinated set of offline, land-only simulations forced by hourly atmospheric fields from the ERA5 reanalysis. An experiment using interannually varying LAI (SENS) is compared with a control simulation based on climatological LAI (CTRL) in order to quantify vegetation feedbacks and their impact on simulated near-surface soil moisture.
Our results show that interannually varying LAI substantially affects near-surface soil moisture anomalies across all three models and over the same water-limited regions. However, the response differs markedly among models. Compared with ESA-CCI observations, near-surface soil moisture anomalies significantly improve in one model (HTESSEL–LPJ-GUESS), whereas the other two models (ECLand and ISBA–CTRIP) exhibit a significant degradation in anomaly correlation. The improved performance in HTESSEL–LPJ-GUESS is attributed to the activation of a positive soil moisture–vegetation feedback enabled by its effective vegetation cover (EVC) parameterization. In HTESSEL–LPJ-GUESS, EVC varies dynamically with LAI following an exponential relationship constrained by satellite observations. Enhanced (reduced) soil moisture limitation during dry (wet) periods leads to negative (positive) LAI and EVC anomalies, which in turn generate a dominant positive feedback on near-surface soil moisture by increasing (decreasing) bare-soil exposure to direct evaporation from the surface. In contrast, ECLand and ISBA–CTRIP prescribe EVC as a fixed parameter that does not respond to LAI variability, preventing the activation of this positive feedback. In these models, the only active feedback on near-surface soil moisture anomalies is negative and arises from reduced (enhanced) transpiration associated with negative (positive) LAI anomalies.
Our findings demonstrate that simply prescribing observed vegetation properties in LSMs does not guarantee a realistic coupling between vegetation and soil moisture. Instead, it is shown that the explicit representation of the underlying vegetation processes is essential to activate the proper feedback and capture the correct soil moisture response.

How to cite: Alessandri, A., Possega, M., Cherchi, A., Di Carlo, E., Boussetta, S., Balsamo, G., Ardilouze, C., Dayon, G., Catalano, F., Gelsinari, S., Massari, C., and van Oorschot, F.:  Surface Soil Moisture–Vegetation Feedbacks in Water-Limited Regions across Land Surface Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19820, https://doi.org/10.5194/egusphere-egu26-19820, 2026.

The plant litter layer, a critical interface between the atmosphere and soil, regulates energy, water, and carbon exchanges, yet its thermal insulation effects are poorly represented in Earth System Models (ESMs). This omission hampers our ability to accurately simulate the climate-hydrology-ecosystem nexus, particularly in cold regions where soil thermal regimes control freeze-thaw processes, hydrology, and biogeochemical cycles. To address this gap, we integrated a dynamic litter layer with explicit thermal properties into the Noah-MP land surface model. Validation against global flux tower sites confirms significant improvements in simulating soil temperature and moisture.
Our results reveal that litter insulation creates a strong seasonal asymmetry in soil temperatures, inducing a net annual cooling (up to –0.69 °C) by providing stronger summer cooling than winter warming. Furthermore, it fundamentally alters soil freeze-thaw processes (FTP), but with divergent impacts: it delays the freezing end date in permafrost regions while advancing it in seasonally frozen ground, with shifts up to 40 days. The strongest modulation of freezing duration (~100 days) occurs in regions with a mean annual temperature near 10°C. We identify six distinct FTP response modes, controlled by the non-linear interplay between climate, litter thickness, and snow depth. The altered thermal and hydrological states feedback to ecosystem processes, offsetting the greening-driven gains in gross primary productivity by 20.57 ± 3.65 g C m⁻² yr⁻¹ while enhancing forest soil organic carbon stocks by 2.08 ± 0.24 kg C m⁻².
These findings demonstrate that the litter layer is a key biogeophysical mediator, directly coupling vegetation dynamics with soil thermal-hydrological states. Explicitly representing this process in ESMs is therefore essential for advancing the simulation of the carbon-water-energy nexus, improving projections of permafrost thaw, ecosystem feedbacks, and hydrological changes under vegetation greening and climate warming.

How to cite: Huang, P., Wang, G., and Valentini, R.: Representing Plant Litter Insulation in Land Surface Models: A Critical Process for Simulating the Soil Thermal-Hydrological-Ecological Nexus in Cold Regions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22297, https://doi.org/10.5194/egusphere-egu26-22297, 2026.

EGU26-1897 | ECS | Posters on site | EOS4.4

The Unreliable Narrator: LSTM Internal States Fluctuate with Software Environments Despite Robust Predictions 

Ryosuke Nagumo, Ross Woods, and Miguel Rico-Ramirez

Since the robust performance of Long Short-Term Memory (LSTM) networks was established, their physics-awareness and interpretability have become central topics in hydrology. Seminal works (e.g., Lees et al. (2022)) have argued that LSTM internal states spontaneously capture hydrological concepts, and suggested that cell states can represent soil moisture dynamics despite not being explicitly trained on such data. Conversely, more recent studies (e.g., Fuente et al. (2024)) demonstrated that mathematical equifinality causes non-unique LSTM representations with different initialisations.

In this work, we report an arguably more systematic "bug" in the software environment that causes instability in internal states. We initially aimed to investigate how internal states behave differently when trained with or without historical observation data. We encountered this issue while reassembling a computational stack and attempting to replicate the initial results, as the original Docker environment was not preserved. While random seeds have been indicated to lead to different internal state trajectories, we found the computational backend (e.g., changing CUDA versions, PyTorch releases, or dependent libraries) also produces them. These are the findings:

  • In gauged catchments: Discharge predictions remained stable (in one catchment, NSE was 0.88 ± 0.01) across computational environments, yet the internal temporal variations (e.g., silhouette, mean, and std of cell states) fluctuated noticeably.
  • In pseudo-ungauged scenarios: The prediction performance itself became more reliant on the computational environment (in the same catchment, NSE dropped to 0.31 ± 0.15), yet the internal temporal variations of the cell states fluctuated only as much as they did during the gauged scenario.

These findings suggests that instability in the computational environment poses not only a risk of altering interpretability in training (by altering internal states) but also casts doubt on reliability in extrapolation (by altering outputs).

It is worth mentioning that we confirmed this is not a replicability issue; completely identical cell states and predictions are produced when the computational environment, seeds, and training data are held constant. We argue that such stability must be established as a standard benchmark before assigning physical meaning to deep learning internals.

How to cite: Nagumo, R., Woods, R., and Rico-Ramirez, M.: The Unreliable Narrator: LSTM Internal States Fluctuate with Software Environments Despite Robust Predictions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1897, https://doi.org/10.5194/egusphere-egu26-1897, 2026.

EGU26-2771 | Posters on site | EOS4.4

New EGU Manuscript Types: Limitations, Errors, Surprises, and Shortcomings as Opportunities for New Science (LESSONS) 

John Hillier, Ulrike Proske, Stefan Gaillard, Theresa Blume, and Eduardo Queiroz Alves

Moments or periods of struggle not only propel scientists forward, but sharing these experiences can also provide valuable lessons for others. Indeed, the current bias towards only publishing ‘positive’ results arguably impedes scientific progress as mistakes that are not learnt from are simply repeated. Here we present a new article type in EGU journals covering LESSONS learnt to help overcome this publishing bias. LESSONS articles describe the Limitations, Errors, Surprises, Shortcomings, and Opportunities for New Science emerging from the scientific process, including non-confirmatory and null results. Unforeseen complications in investigations, plausible methods that failed, and technical issues are also in scope. LESSONS thus fit the content of the BUGS session and can provide an outlet for articles based on session contributions. Importantly, a LESSONS Report will offer a substantial, valuable insight. LESSONS Reports are typically short (1,000-2,000 words) to help lower the barrier to journal publication, whilst LESSONS Posts (not peer-reviewed, but with a DOI on EGUsphere) can be as short as 500 words to allow early-stage reporting. LESSONS aim to destigmatise limitations, errors, surprises and shortcomings and to add these to the published literature as opportunities for new science – we invite you to share your LESSONS learnt.

 

Finally, a big thank you from this paper’s ‘core’ writing team to the wider group who have helped shape the LESSONS idea since EGU GA in 2025, including PubCom and in particular its Chair Barbara Ervens.

How to cite: Hillier, J., Proske, U., Gaillard, S., Blume, T., and Queiroz Alves, E.: New EGU Manuscript Types: Limitations, Errors, Surprises, and Shortcomings as Opportunities for New Science (LESSONS), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2771, https://doi.org/10.5194/egusphere-egu26-2771, 2026.

EGU26-3077 | ECS | Posters on site | EOS4.4

False Starts and Silver Linings: A Photocatalytic Journey with Layered Double Hydroxides 

Anna Jędras and Jakub Matusik

Photocatalysis is frequently presented in the literature as a straightforward route toward efficient degradation of pollutants, provided that the “right” material is selected. Layered double hydroxides (LDH) are often highlighted as promising photocatalysts due to their tunable composition and reported activity in dye degradation. Motivated by these claims, this study evaluated LDH as mineral analogs for photocatalytic water treatment, ultimately uncovering a series of unexpected limitations, methodological pitfalls, and productive surprises.

In the first stage, Zn/Cr, Co/Cr, Cu/Cr, and Ni/Cr LDHs were synthesized and tested for photocatalytic degradation of methylene blue (0.02 mM) and Acid Blue Dye 129 (0.3 mM). Contrary to expectations,1 photocatalytic performance was consistently low. After one hour of irradiation, concentration losses attributable to photocatalysis did not exceed 15%, while most dye removal resulted from adsorption. Despite extensive efforts to optimize synthesis protocols, catalyst composition, and experimental conditions, this discrepancy with previously published studies could not be resolved.

To overcome limitations related to particle dispersion, surface accessibility, and charge-carrier separation, a second strategy was pursued by incorporating clay minerals as supports.2 Zn/Cr LDH, identified as the most active composition in preliminary tests, was coprecipitated with kaolinite, halloysite, and montmorillonite. Experiments with methylene blue (0.1 mM) and Acid Blue 129 (0.3 mM) demonstrated enhanced adsorption capacities. However, photocatalytic degradation efficiencies remained poor, typically below 10% after one hour, indicating that apparent performance gains were largely adsorption-driven rather than photochemical.

This failure proved to be a turning point. Instead of abandoning LDH entirely, they were combined with graphitic carbon nitride (GCN) to form a heterostructure.3 This approach resulted in a dramatic improvement: after optimization of the synthesis protocol, 99.5% of 1 ppm estrone was degraded within one hour.4 Further modifications were explored by introducing Cu, Fe, and Ag into the LDH/GCN system. While Cu and Fe suppressed photocatalytic activity, silver, at an optimized loading, reduced estrone concentrations below the detection limit within 40 minutes.5

This contribution presents a full experimental arc - from promising hypotheses that failed, through misleading adsorption-driven “successes,” to an ultimately effective but non-intuitive solution - highlighting the value of negative results and surprises as drivers of scientific progress.

This research was funded by the AGH University of Krakow, grant number 16.16.140.315.

Literature:

1            N. Baliarsingh, K. M. Parida and G. C. Pradhan, Ind. Eng. Chem. Res., 2014, 53, 3834–3841.

2            A. Í. S. Morais, W. V. Oliveira, V. V. De Oliveira, L. M. C. Honorio, F. P. Araujo, R. D. S. Bezerra, P. B. A. Fechine, B. C. Viana, M. B. Furtini,
              E. C. Silva-Filho and J. A. Osajima, Journal of Environmental Chemical Engineering, 2019, 7, 103431.

3            B. Song, Z. Zeng, G. Zeng, J. Gong, R. Xiao, S. Ye, M. Chen, C. Lai, P. Xu and X. Tang, Advances in Colloid and Interface Science, 2019, 272, 101999.

4            A. Jędras, J. Matusik, E. Dhanaraman, Y.-P. Fu and G. Cempura, Langmuir, 2024, 40, 18163–18175.

5            A. Jędras, J. Matusik, J. Kuncewicz and K. Sobańska, Catal. Sci. Technol., 2025, 15, 6792–6804.

How to cite: Jędras, A. and Matusik, J.: False Starts and Silver Linings: A Photocatalytic Journey with Layered Double Hydroxides, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3077, https://doi.org/10.5194/egusphere-egu26-3077, 2026.

EGU26-4074 | Orals | EOS4.4

Instructive surprises in the hydrological functioning of landscapes 

James Kirchner, Paolo Benettin, and Ilja van Meerveld

BUGS can arise in individual research projects, but also at the level of communities of researchers, leading to shifts in the scientific consensus.  These community-level BUGS typically arise from observations that are surprising to (or previously overlooked by) substantial fractions of the research community.  In this presentation, we summarize several community-level BUGS in our field: specifically, key surprises that have transformed the hydrological community's understanding of hillslope and catchment processes in recent decades.  

Here are some examples.  (1) Students used to learn (and some still do today) that storm runoff is dominated by overland flow.  But stable isotope tracers have convincingly shown instead that even during storm peaks, streamflow is composed mostly of water that has been stored in the landscape for weeks, months, or years.  (2) Maps, and most hydrological theories, have typically depicted streams as fixed features of the landscape.  But field mapping studies have shown that stream networks are surprisingly dynamic, with up to 80% of stream channels going dry sometime during the year.  (3) Textbooks have traditionally represented catchment storage as a well-mixed box.  But tracer time series show fractal scaling that cannot be generated by well-mixed boxes, forcing a re-think of our conceptualization of subsurface storage and mixing.  (4) Waters stored in aquifers, and the waters that drain from them, have traditionally been assumed to share the same age.  But tracers show that waters draining from aquifers are often much younger than the groundwaters that are left behind, and this was subsequently shown to be an inevitable result of aquifer heterogeneity. 

Several examples like these, and their implications, will be briefly discussed, with an eye to the question: how can we maximize the chances for future instructive surprises?

How to cite: Kirchner, J., Benettin, P., and van Meerveld, I.: Instructive surprises in the hydrological functioning of landscapes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4074, https://doi.org/10.5194/egusphere-egu26-4074, 2026.

Coming from geosciences, we hopefully know what we want to do. Coming from numerics, however, we often know quite well what we are able to do and look for a way to sell it to the community. A few years ago, deep-learning techniques brought new life into the glaciology community. These approaches  allowed for simulations of glacier dynamics at an unprecedented computational performance and motivated several researchers to tackle the numerous open questions about past and present glacier dynamics, particularly in alpine regions. From another point of view, however, it was also tempting to demonstrate that the human brain is still more powerful than artificial intelligence by developing a new classical numerical scheme that can compete with deep-learning techniques concerning its efficiency.

Starting point was, of course, the simplest approximation to the full 3-D Stokes equations, the so-called shallow ice approximation (SIA). Progress was fast and the numerical performance was even better than expected. The new numerical scheme enabled simulations with spatial resolutions of 25 m on a desktop PC, while previous schemes did not reach simulations below a few hundred meters.

However, the enthusiasm pushed the known limitations of the SIA a bit out of sight. Physically, the approximation is quite bad on rugged terrain, particularly in narrow valleys. So the previous computational limitations have been replaced by physical limitations since high resolutions are particularly useful for rugged topographies. In other words, a shabby house has a really good roof now.

What are the options in such a situation?

  • Accept that there is no free lunch and avoid contact to the glacialogy community in the future.
  • Continue the endless discussion about the reviewers' opinion that a spatial resolution of 1 km is better than 25 m.
  • Find a real-world data set that matches the results of the model and helps to talk the problems away.
  • Keep the roof and build a new house beneath. Practically, this would be developing a new approximation to the full 3-D Stokes equations that is compatible to the numerical scheme and reaches an accuracy similar to those of the existing approximations.
  • Take the roof and put it on one of the existing solid houses. Practically, this would be an extension of the numerical scheme towards more complicated systems of differential equations. Unfortunately, efficient numerical schemes are typically very specific. So the roof will not fit easily and it might leak.

The story is open-ended, but there will be at least a preliminary answer in the presentation.

 

How to cite: Hergarten, S.: How useful is a new roof on a shabby house? An example from glacier modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4196, https://doi.org/10.5194/egusphere-egu26-4196, 2026.

EGU26-4587 | Posters on site | EOS4.4

The importance of describing simple methods in climate sensitivity literature 

Anna Zehrung, Andrew King, Zebedee Nicholls, Mark Zelinka, and Malte Meinshausen

“Show your working!” – is the universal phrase drilled into science and maths students to show a clear demonstration of the steps and thought processes used to reach a solution (and to be awarded full marks on the exam). 

Beyond the classroom, “show your working” becomes the methods section on every scientific paper, and is critical for the transparency and replicability of the study. However, what happens if parts of the method are considered assumed knowledge, or cut in the interests of a word count? 

An inability to fully replicate the results of a study became the unexpected glitch at the start of my PhD. Eager to familiarise myself with global climate model datasets, I set out to replicate the results of a widely cited paper which calculates the equilibrium climate sensitivity (ECS) across 27 climate models. The ECS is the theoretical global mean temperature response to a doubling of atmospheric CO2 relative to preindustrial levels. A commonly used method to calculate the ECS is to apply an ordinary least squares regression to global annual mean temperature and radiative flux anomalies. 

Despite the simplicity of a linear regression between two variables, we obtained ECS estimates for some climate models that differed from those reported in the original study, even though we followed the described methodology. However, the methodology provided only limited detail on how the raw climate model output – available at regional and monthly scales – was processed to obtain global annual mean anomalies. Differences in these intermediate processing steps can, in turn, lead to differences in ECS estimates.

Limited reporting of data-processing steps is common in the ECS literature. Whether these steps are considered assumed knowledge or deemed too simple to warrant explicit description, we demonstrate that, for some models, they can materially affect the resulting ECS estimate. While the primary aim of our study is to recommend a standardised data-processing pathway for ECS calculations, a secondary aim is to highlight the lack of transparency in key methodological details across the literature. A central takeaway is the importance of clearly documenting all processing steps – effectively, to “show your working” – and to emphasise the critical role of a detailed methods section.

How to cite: Zehrung, A., King, A., Nicholls, Z., Zelinka, M., and Meinshausen, M.: The importance of describing simple methods in climate sensitivity literature, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4587, https://doi.org/10.5194/egusphere-egu26-4587, 2026.

Observation of atmospheric constituents and processes is not easy. As atmospheric chemists, we use sensitive equipment, for example mass spectrometers, that we often set up in a (remote) location or on a moving platform for a few-weeks campaign to make in-situ observations. All this with the goal of explaining more and more atmospheric processes, and to verify and improve atmospheric models. However, glitches can happen anywhere in an experiment, be it in the experimental design, setup, or instrumental performance. Thus, complete data coverage during such a campaign is not always a given, resulting in gaps in (published) datasets. And the issue with air is that you can never go back and measure the exact same air again. Here, I would like to share some stories behind such gaps, and what we learned from them. This presentation aims to encourage early career researchers who might be struggling with feelings of failure when bugs, blunders and glitches happen in their experiments - you are not alone! I will share what we learned from these setbacks and how each of them improved our experimental approaches.

How to cite: Pfannerstill, E. Y.: Why are there gaps in your measurements? Sharing the stories behind the missing datapoints, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5494, https://doi.org/10.5194/egusphere-egu26-5494, 2026.

Over a 24-year research period, three successive experimental investigations led to three publications, each of which falsified the author’s preceding hypothesis and proposed a revised conceptual framework. Despite an initial confidence in having identified definitive solutions, subsequent experimental evidence consistently demonstrated the limitations and inaccuracies of earlier interpretations. This iterative process ultimately revealed that samples, in particular geological reference materials, sharing identical petrographic or mineralogical descriptions are not necessarily chemically equivalent and can exhibit markedly different behaviors during chemical digestion procedures. These findings underscore the critical importance of continuous hypothesis testing, self-falsification, and experimental verification in scientific research, particularly when working with reference materials assumed to be identical. I will be presenting data on the analysis of platinum group elements (PGE) and osmium isotopes in geological reference materials (chromitites, ultramafic rocks and basalts), which demonstrates the need for challenging matrices for method validation. 

How to cite: Meisel, T. C.: Self-falsification as a driver of scientific progress: Insights from long-term experimental research, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5771, https://doi.org/10.5194/egusphere-egu26-5771, 2026.

EGU26-6794 | ECS | Orals | EOS4.4

Back to square one (again and again): Finding a bug in a complex global atmospheric model   

Nadja Omanovic, Sylvaine Ferrachat, and Ulrike Lohmann

In atmospheric sciences, a central tool to test hypotheses are numerical models, which aim to represent (part of) our environment. One such model is the weather and climate model ICON [1], which solves the Navier-Stokes equation for capturing the dynamics and parameterizes subgrid-scale processes, such as radiation, cloud microphysics, and aerosol processes. Specifically, for the latter exists the so-called Hamburg Aerosol Module (HAM [2]), which is coupled to ICON [3] and predicts the evolution of aerosol populations using two moments (mass mixing ratio and number concentration). The high complexity of aerosols is reflected in the number of aerosol species (total of 5), number of modes (total of 4), and their mixing state and solubility. The module calculates aerosol composition and number concentration, their optical properties, their sources and sinks, and their interactions with clouds via microphysical processes. Aerosol emissions are sector-specific and based on global emission inventories or dynamically computed.

Within our work, we stumbled upon an interesting pattern occurrence in our simulations upon changing/turning off single emission sectors. If we, e.g., removed black carbon from aircraft emissions, the strongest changes emerged over the African continent, which is not the region where we were expecting to see the strongest response. Further investigations revealed that this pattern emerges independently of the emission sector as well as species, confirming our suspicion that we are facing a bug within HAM. Here, we want to present how we approached the challenge of identifying and tackling a bug within a complex module with several thousand lines of code.

 

[1] G. Zängl, D. Reinert, P. Ripodas, and M. Baldauf, “The ICON (ICOsahedral Non-hydrostatic) modelling framework of DWD and MPI-M: Description of the non-hydrostatic dynamical core,” Quarterly Journal of the Royal Meteorological Society, vol. 141, no. 687, pp. 563–579, 2015, ISSN: 1477-870X. DOI: 10.1002/qj.2378

[2] P. Stier, J. Feichter, S. Kinne, S. Kloster, E. Vignati, J. Wilson, L. Ganzeveld, I. Tegen, M. Werner, Y. Balkanski, M. Schulz, O. Boucher, A. Minikin, and A. Petzold, “The aerosol-climate model ECHAM5-HAM,” Atmospheric Chemistry and Physics, 2005. DOI: 10.5194/acp-5-1125-2005

[3] M. Salzmann, S. Ferrachat, C. Tully, S. M¨ unch, D. Watson-Parris, D. Neubauer, C. Siegenthaler-Le Drian, S. Rast, B. Heinold, T. Crueger, R. Brokopf, J. Mülmenstädt, J. Quaas, H. Wan, K. Zhang, U. Lohmann, P. Stier, and I. Tegen, “The Global Atmosphere-aerosol Model ICON-A-HAM2.3–Initial Model Evaluation and Effects of Radiation Balance Tuning on Aerosol Optical Thickness,” Journal of Advances in Modeling Earth Systems, vol. 14, no. 4,e2021MS002699, 2022, ISSN: 1942-2466. DOI: 10.1029/2021MS002699

How to cite: Omanovic, N., Ferrachat, S., and Lohmann, U.: Back to square one (again and again): Finding a bug in a complex global atmospheric model  , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6794, https://doi.org/10.5194/egusphere-egu26-6794, 2026.

In situ cloud measurements are essential for understanding atmospheric processes and establishing a reliable ground truth. Obtaining these data is rarely straightforward. Challenges range from accessing clouds in the first place to ensuring that the instrument or environment does not bias the sample. This contribution explores several blunders and unexpected glitches encountered over fifteen years of field campaigns.

I will share stories of mountain top observations where blowing snow was measured instead of cloud ice crystals and the ambitious but failed attempt to use motorized paragliders for sampling. I also reflect on winter campaigns where the primary obstacles were flooding and mud rather than cold and snow. While these experiences were often frustrating, they frequently yielded useful data or led to new insights. One such example is the realization that drone icing is not just a crash risk but can also serve as a method for measuring liquid water content. By highlighting these setbacks and the successful data that emerged despite them, I aim to foster a discussion on the value of trial and error and persistence in atmospheric physics.

How to cite: Henneberger, J.: How Not to Measure a Cloud: Lessons from Fifteen Years of Fieldwork Failures, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8228, https://doi.org/10.5194/egusphere-egu26-8228, 2026.

EGU26-8359 | ECS | Posters on site | EOS4.4

Do trees save lives under climate change? It’s complicated  

Nils Hohmuth, Nora L. S. Fahrenbach (presenting), Yibiao Zou (presenting), Josephine Reek, Felix Specker, Tom Crowther, and Constantin M. Zohner

Forests are powerful climate regulators: Their CO2 uptake provides a global biogeochemical cooling effect, and in the tropics, this cooling is further strengthened by evapotranspiration. Given that temperature-related mortality is a relevant global health burden, which is expected to increase under climate change, we set out to test what we thought was a promising hypothesis: Can forests reduce human temperature-related mortality from climate change? 

To test this, we used simulated temperature changes to reforestation from six different Earth System Models (ESMs) under a future high-emission scenario, and paired them with age-specific population data and three methodologically different temperature-mortality frameworks (Cromar et al. 2022, Lee et al. 2019, and Carleton et al. 2022). We expected to find a plausible range of temperature-related mortality outcomes attributable to global future forests conservation efforts.

Instead, our idea ran head-first into a messy reality. Firstly, rather than showing a clear consensus, the ESMs produced a wide range of temperature responses to reforestation, varying both in magnitude and sign. This is likely due to the albedo effect, varying climatological tree cover and land use processes implemented by the models, in addition to internal variability which we could not reduce due to the existence of only one ensemble member per model. Consequently, the models disagreed in many regions on whether global forest conservation and reforestation would increase or decrease temperature by the end of the century.

The uncertainties deepened when we incorporated the mortality data. Mortality estimates varied by up to a factor of 10 depending on the ESM and mortality framework used. Therefore, in the end, the models could not even agree on whether forests increased or decreased temperature-related mortality. We found ourselves with a pipeline that amplified uncertainties of both the ESM and mortality datasets.

For now, the question remains wide open: Do trees save us from temperature-related deaths in a warming world, and if so, by how much?

 

* The first two authors contributed equally to this work.

How to cite: Hohmuth, N., Fahrenbach (presenting), N. L. S., Zou (presenting), Y., Reek, J., Specker, F., Crowther, T., and Zohner, C. M.: Do trees save lives under climate change? It’s complicated , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8359, https://doi.org/10.5194/egusphere-egu26-8359, 2026.

EGU26-10401 | ECS | Orals | EOS4.4

The empty mine: Why better tools do not help you find new diamonds 

Ralf Loritz, Alexander Dolich, and Benedikt Heudorfer

Hydrological modelling has long been shaped by a steady drive toward ever more sophisticated models. In the era of machine learning, this race has turned into a relentless pursuit of complexity: deeper networks and ever more elaborate architectures that often feel outdated by the time the ink on the paper is dry. Motivated by a genuine belief in methodological progress, I, like many others, spent considerable effort exploring this direction, driven by the assumption that finding the “right” architecture or model would inevitably lead to better performance. This talk is a reflection on that journey; you could say my own Leidensweg. Over several years, together with excellent collaborators, I explored a wide range of state-of-the-art deep-learning approaches for rainfall–runoff modelling and other hydrological modelling challenges. Yet, regardless of the architecture or training strategy, I repeatedly encountered the same performance ceiling. In parallel, the literature appeared to tell a different story, with “new” models regularly claiming improvements over established baselines. A closer inspection, however, revealed that rigorous and standardized benchmarking is far from common practice in hydrology, making it difficult to disentangle genuine progress from artefacts of experimental design. What initially felt like a failure to improve my models turned out to be a confrontation with reality. The limiting factor was not the architecture, but the problem itself. We have reached a point where predictive skill is increasingly bounded by the information content of our benchmark datasets and maybe more importantly by the way we frame our modelling challenges, rather than by model design. Like many others, I have come to believe that if we want to move beyond the current performance plateau, the next breakthroughs are unlikely to come from ever more complex models alone. Instead, as a community, we need well-designed model challenges, better benchmarks, and datasets that meaningfully expand the information available to our models to make model comparisons more informative.

How to cite: Loritz, R., Dolich, A., and Heudorfer, B.: The empty mine: Why better tools do not help you find new diamonds, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10401, https://doi.org/10.5194/egusphere-egu26-10401, 2026.

EGU26-13630 | ECS | Orals | EOS4.4

How NOT to identify streamflow events? 

Larisa Tarasova and Paul Astagneau

Examining catchment response to precipitation at event scale is useful for understanding how various hydrological systems store and release water. Many of such event scale characteristics, for example event runoff coefficient and event time scale are also important engineering metrics used for design. However, deriving these characteristics requires identification of discrete precipitation-streamflow events from continuous hydrometeorological time series.

Event identification is not at all a trivial task. It becomes even more challenging when working with very large datasets that encompass a wide range of spatial and temporal dynamics. Approaches range from visual expert judgement to baseflow-separation-based methods and objective methods based on the coupled dynamics of precipitation and streamflow. Here, we would like to present our experience in the quest to devise the “ideal” method for large datasets – and trust us, we tried, a lot. We demonstrate that expert-based methods can be seriously flawed simply by changing a few meta parameters, such as the length of displayed periods, baseflow-separation-based methods deliver completely opposite results when different underlying separation methods are selected, and objective methods suddenly fail when dynamics with different temporal scales are simultaneously present.

Ultimately, we realized that finding a one-size-fits-all method was not possible and that compromises had to be made to select sufficiently representative events across large datasets. Therefore, we advocate for pragmatic case-specific evaluation criteria and for transparency in event identification to make study results reproducible and fit for purpose, if not perfect.

How to cite: Tarasova, L. and Astagneau, P.: How NOT to identify streamflow events?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13630, https://doi.org/10.5194/egusphere-egu26-13630, 2026.

EGU26-14148 | Orals | EOS4.4 | Highlight

Buggy benefits of more fundamental climate models 

Bjorn Stevens, Marco Giorgetta, and Hans Segura

A defining attribute of global-storm resolving models is that modelling is replaced by simulation.  In addition to overloading the word “model”  this avails the developer of a much larger variety of tests, and brings about a richer interplay with their intuition.  This has proven helpful in identifying and correcting many mistakes in global-storm resolving models that traditional climate models find difficult to identify, and usually compensate by “tuning.”  It also means that storm-resolving models are built and tested in a fundamentally different way than are traditional climate models. In this talk I will review the development of ICON as a global storm resolving model to illustrate how this feature, of trying to simulate rather than model the climate system, has helped identify a large number of long-standing bugs in code bases inherited from traditional models; how this can support open development; and how sometimes these advantages also prove to be buggy.

How to cite: Stevens, B., Giorgetta, M., and Segura, H.: Buggy benefits of more fundamental climate models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14148, https://doi.org/10.5194/egusphere-egu26-14148, 2026.

EGU26-14374 | Orals | EOS4.4

The dangerous temptation of optimality in hydrological and water resources modelling 

Thorsten Wagener and Francesca Pianosi

Hydrological and water systems modelling has long been driven by the search for better models. We do so by searching for models or at least parameter combinations that provide the best fit to given observations. We ourselves have contributed to this effort by developing new methods and by publishing diverse case studies. However, we repeatedly find that searching for and finding an optimal model is highly fraught in the presence of unclear signal-to-noise ratios in our observations, of incomplete models and of highly imbalanced databases. We present examples of our own work through which we have realized that achieving optimality was possible but futile unless we give equal consideration to issues of consistency, robustness and problem framing. We argue here that the strong focus on optimality continues to be a hindrance for advancing hydrologic science and for transferring research achievements into practice – probably more so than in other areas of the geosciences.

How to cite: Wagener, T. and Pianosi, F.: The dangerous temptation of optimality in hydrological and water resources modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14374, https://doi.org/10.5194/egusphere-egu26-14374, 2026.

Among soil physical analyses, determination of the soil particle-size distribution (PSD) is arguably the most fundamental. The standard methodology combines sieve analysis for sand fractions with sedimentation-based techniques for silt and clay. Established sedimentation methods include the pipette and hydrometer techniques. More recently, the Integral Suspension Pressure (ISP) method has become available, which derives PSD by inverse modeling of the temporal evolution of suspension pressure measured at a fixed depth in a sedimentation cylinder. Since ISP is based on the same physical principles as the pipette and hydrometer methods, their results should, in principle, agree.

The ISP methodology has been implemented in the commercial instrument PARIO (METER Group, Munich). While elegant, the method relies on pressure change measurements with a resolution of 0.1 Pa (equivalent to 0.01 mm of water column). Consequently, the PARIO manual strongly advises avoiding any mechanical disturbance such as thumping, bumping, clapping, vibration, or other shock events. This warning is essentially precautionary, because to date no systematic experimental investigation of such disturbances has been reported.

To explore this issue, we prepared a single 30 g soil sample following standard PSD procedures and subjected it to 26 PARIO repeated measurement runs over a period of five months, each run lasting 12 h. Between runs, the suspension was remixed but otherwise not altered. The first ten runs (over ten days) were conducted without intentional disturbance to establish baseline repeatability. This was followed by eight runs with deliberately imposed and timed disturbances that generated single or repeated vibrations (“rocking and shocking”). After approximately two and five months, we conducted additional sets of five and three undisturbed runs, respectively.

We report how these mechanical disturbances, along with temperature variations during measurement and the time elapsed since sample pre-treatment, affected the derived PSD. The results provide a first quantitative assessment of how fragile—or robust—the ISP method and PARIO system really are when reality refuses to sit perfectly still.

 

How to cite: Nemes, A. and Durner, W.: Rocking and Shocking the PARIOTM: How Sensitive Is ISP-Based Particle-Size Analysis to Mechanical Disturbance?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14763, https://doi.org/10.5194/egusphere-egu26-14763, 2026.

EGU26-14852 | Posters on site | EOS4.4

Some Norwegian soils behave differently: is it an inheritance from marine sedimentation? 

Attila Nemes, Pietro Bazzocchi, Sinja Weiland, and Martine van der Ploeg

Predicting soil hydraulic behavior is necessary for the modeling of catchments and agricultural planning, particularly for a country like Norway where only 3% of land is suitable for farming. Soil texture is an important and easily accessible parameter for the prediction of soil hydraulic behavior. However, some Norwegian farmland soils, which formed as glacio-marine sediments and are characterized by a medium texture, have shown the hydraulic behavior of heavy textured soils. Coined by the theory behind well-established sedimentation-enhancing technology used in waste water treatment, we hypothesized that sedimentation under marine conditions may result in specific particle sorting and as a result specific pore system characteristics. To test this, we designed four custom-built devices to produce artificially re-sedimented columns of soil material to help characterize the influence of sedimentation conditions. We successfully produced column samples of the same homogeneous mixture of fine-sand, silt, and clay particles obtained by physically crushing and sieving (< 200 µm) subsoil material collected at the Skuterud catchment in South-East Norway, differing only in sedimentation conditions (deionized water vs 35 g per liter NaCl solution). Then, the inability of standard laboratory methods to measure the saturated hydraulic conductivity of such fine material, led us to “MacGyver” (design and custom-build) two alternative methodologies to measure that property, i.e. i) by adapting a pressure plate extractor for a constant head measurement and ii) by building a 10 m tall pipe-system in a common open area of the office, in order to increase the hydraulic head on the samples. There was a learning curve with both of those methods, but we have found that the salt-water re-sedimented columns were about five times more permeable than the freshwater ones, which was the complete opposite of our expectations. However, an unexpected blunder in the conservation of our samples suggests that our hypothesis should be further explored rather than dismissed. These contributions hint about the mechanisms that may underlie the anomalous hydraulic behaviour of certain Norwegian soils and raise new questions on the formation of marine clays, improving knowledge available for land managers and modellers.

 

How to cite: Nemes, A., Bazzocchi, P., Weiland, S., and van der Ploeg, M.: Some Norwegian soils behave differently: is it an inheritance from marine sedimentation?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14852, https://doi.org/10.5194/egusphere-egu26-14852, 2026.

EGU26-16619 | Orals | EOS4.4

The unknown knowns – the inconvenient knowledge in hydrogeology we do not like to use 

Okke Batelaan, Joost Herweijer, Steven Young, and Phil Hayes

“It is in the tentative stage that the affections enter with their blinding influence. Love was long since represented as blind…The moment one has offered an original explanation for a phenomenon which seems satisfactory, that moment affection for his intellectual child springs into existence…To guard against this, the method of multiple working hypotheses is urged. … The effort is to bring up into view every rational explanation of new phenomena, and to develop every tenable hypothesis respecting their cause and history. The investigator thus becomes the parent of a family of hypothesis: and, by his parental relation to all, he is forbidden to fasten his affections unduly upon any one” (Chamberlin, 1890).

The MADE (macro-dispersion) natural-gradient tracer field experiments were conducted more than 35 years ago. It aimed to determine field-scale dispersion parameters based on detailed hydraulic conductivity measurements to support transport simulation. A decade of field experiments produced a 30-year paper trail of modelling studies with no clear resolution of a successful simulation approach for practical use in transport problems.  As a result, accurately simulating contaminant transport in the subsurface remains a formidable challenge in hydrogeology.

What went awry, and why do we often miss the mark?

Herweijer et al. (2026) conducted a ‘back to basics’ review of the original MADE reports and concluded that there are significant inconvenient and unexplored issues that influenced the migration of the tracer plume and or biased observations. These issues include unreliable measurement of hydraulic conductivity, biased tracer concentrations, and underestimation of sedimentological heterogeneity and non-stationarity of the flow field. Many studies simulating the tracer plumes appeared to have ignored, sidestepped, or been unaware of these issues, raising doubts about the validity of the results.

Our analysis shows that there is a persistent drive among researchers to conceptually oversimplify natural complexity to enable testing of single-method modelling, mostly driven by parametric stochastic approaches. Researchers tend to be anchored to a specialised, numerically driven methodology and have difficulty in unearthing highly relevant information from ‘unknown known’ data or applying approaches outside their own specialised scientific sub-discipline. Another important aspect of these ‘unkowns knowns’ is the tendency to accept published data verbatim. Too often, there is no rigorous investigation of the original measurement methods and reporting, and, if need be, additional testing to examine the root cause of data issues.

Following the good old advice of Chamberlin (1890), we used a knowledge framework to systematically assess knowns, unknowns, and associated confidence levels, yielding a set of multi-conceptual models. Based on identified 'unknowns', these multi-models can be tested against reliable 'knowns' such as piezometric data and mass balance calculations.  

Chamberlin, T.C., 1890, The method of multiple working hypotheses. Science 15(366): 92-96. doi:10.1126/science.ns-15.366.92.

Herweijer J.C., S. C Young, P. Hayes, and O. Batelaan, 2026, A multi-conceptual model approach to untangling the MADE experiment, Accepted for Publication in Groundwater.

How to cite: Batelaan, O., Herweijer, J., Young, S., and Hayes, P.: The unknown knowns – the inconvenient knowledge in hydrogeology we do not like to use, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16619, https://doi.org/10.5194/egusphere-egu26-16619, 2026.

EGU26-17373 | Posters on site | EOS4.4

The Hidden Propagator: How Free-Slip Boundaries Corrupt 3D Simulations 

Laetitia Le Pourhiet

Free-slip boundary conditions are routinely used in 3D geodynamic modelling because they reduce computational cost, avoid artificial shear zones at domain edges, and simplify the implementation of large-scale kinematic forcing. However, despite their apparent neutrality, our experiments show that free-slip boundaries systematically generate first-order artefacts that propagate deep into the model interior and can severely distort the interpretation of continental rifting simulations.

Here we present a set of 3D visco-plastic models inspired by the South China Sea (SCS) that were originally designed to study the effect of steady-state thermal inheritance and pluton-controlled crustal weakening. Unexpectedly, in all simulations except those with a very particular inverted rheological profile (POLC), the free-slip boundary on the “Vietnam side” of the domain generated a persistent secondary propagator, producing unrealistic amounts of lithospheric thinning in the southwest corner. This artefact appeared irrespective of crustal rheology, seeding strategy, or the presence of thermal heterogeneities.

We identify three systematic behaviours induced by free-slip boundaries in 3D:
(1) forced rift nucleation at boundary-adjacent thermal gradients,
(2) artificial propagator formation that competes with the intended first-order rifting, and
(3) rotation or shearing of micro-blocks not predicted by tectonic reconstructions.

These artefacts originate from the inability of free-slip boundaries to transmit shear traction, which artificially channels deformation parallel to the boundary when lateral thermal or mechanical contrasts exist. In 3D, unlike in 2D, the combination of oblique extension and boundary-parallel velocity freedom leads to emergent pseudo-transform behaviour that is entirely numerical.

Our results highlight a key negative outcome: free-slip boundaries cannot be assumed neutral in 3D rift models, especially when studying localisation, obliquity, multi-propagator dynamics, or the competition between structural and thermal inheritance. We argue that many published 3D rift models may unknowingly include such artefacts.

 

How to cite: Le Pourhiet, L.: The Hidden Propagator: How Free-Slip Boundaries Corrupt 3D Simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17373, https://doi.org/10.5194/egusphere-egu26-17373, 2026.

EGU26-18600 | Posters on site | EOS4.4

Data Disaster to Data Resilience: Lessons from CEDA’s Data Recovery  

Edward Williamson, Matt Pritchard, Alan Iwi, Sam Pepler, and Graham Parton

On 18 November 2025, a small error during internal data migration of between storage systems of the JASMIN data analysis platform in the UK led to a substantial part of the CEDA Archive being made temporarily unavailable online (but not lost!). The unfortunate incident caused serious disruption to a large community of users (and additional workload and stress for the team), it provided important learning points for the team in terms of:  

  • enhancing data security,  
  • importance of mutual support among professional colleagues,  
  • the value of clear and transparent communications with your users 
  • a unique opportunity to showcase the capabilities of a cutting-edge digital research infrastructure in the recovery and return to service with this “unscheduled disaster recovery exercise”. 

 

We report on the circumstances leading to the incident, the lessons learned, and the technical capabilities employed in the recovery. One example shows, nearly 800 Terabytes of data transferred from a partner institution in the USA in just over 27 hours, at a rate of over 8 Gigabytes per second using Globus. The ability to orchestrate such a transfer is the result of many years of international collaboration to support large-scale environmental science, and highlights the benefits of a federated, replicated data infrastructure built on well-engineered technologies.

How to cite: Williamson, E., Pritchard, M., Iwi, A., Pepler, S., and Parton, G.: Data Disaster to Data Resilience: Lessons from CEDA’s Data Recovery , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18600, https://doi.org/10.5194/egusphere-egu26-18600, 2026.

EGU26-19755 | ECS | Posters on site | EOS4.4

Opposite cloud responses to extreme Arctic pollution: sensitivity to cloud microphysics, or a bug? 

Rémy Lapere, Ruth Price, Louis Marelle, Lucas Bastien, and Jennie Thomas

Aerosol-cloud interactions remain one of the largest uncertainties in global climate modelling. This uncertainty arises because of the dependence of aerosol-cloud interactions on many tightly coupled atmospheric processes; the non-linear response of clouds to aerosol perturbations across different regimes; and the challenge of extracting robust signals from noisy meteorological observations. The problem is particularly acute in the Arctic, where sparse observational coverage limits model constraints, pristine conditions can lead to unexpected behaviour, and key processes remain poorly understood.

A common way to tackle the challenge of uncertainties arising from aerosol-cloud interactions in climate simulations is to conduct sensitivity experiments using cloud and aerosol microphysics schemes based on different assumptions and parameterisations. By comparing these experiments, key results can be constrained by sampling the range of unavoidable structural uncertainties in the models. Here, we apply this approach to a case study of an extreme, polluted warm air mass in the Arctic that was measured during the MOSAiC Arctic expedition in 2020. We simulated the event in the WRF-Chem-Polar regional climate model both with and without the anthropogenic aerosols from the strong pollution event to study the response of clouds and surface radiative balance. To understand the sensitivity of our results to the choice of model configuration, we tested two distinct, widely-used cloud microphysics schemes.

Initial results showed that the two schemes simulated opposite cloud responses: one predicted a surface cooling from the pollution that was reasonably in line with our expectations of the event, while the other predicted the opposite behaviour in the cloud response and an associated surface warming. These opposing effects seemed to suggest that structural uncertainties in the two schemes relating to clean, Arctic conditions was so strong that it even obscured our ability to understand the overall sign of the surface radiative response to the pollution.

However, since significant model development was required to couple these two cloud microphysics schemes to the aerosol fields in our model, there was another explanation that we couldn’t rule out: a bug in the scheme that was producing the more unexpected results. In this talk, we will explore the challenges of simulating the Arctic climate with a state-of-the-art chemistry-climate model and highlight how examples like this underscore the value of our recent efforts to align our collaborative model development with software engineering principles and Open Science best practices.

How to cite: Lapere, R., Price, R., Marelle, L., Bastien, L., and Thomas, J.: Opposite cloud responses to extreme Arctic pollution: sensitivity to cloud microphysics, or a bug?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19755, https://doi.org/10.5194/egusphere-egu26-19755, 2026.

All statistical tools come with assumptions. Yet many scientists treat statistics like a collection of black-box methods without learning the assumptions. Here I illustrate this problem using dozens of studies that claim to show that solar variability is a dominant driver of climate. I find that linear regression approaches are widely misused among these studies. In particular, they often violate the assumption of ‘no autocorrelation’ of the time series used, though it is common for studies to violate several or all of the assumptions of linear regression. The misuse of statistical tools has been a common problem across all fields of science for decades. This presentation serves as an important cautionary tale for the Earth Sciences and highlights the need for better statistical education and for statistical software that automatically checks input data for assumptions.

How to cite: Steiger, N.: Pervasive violation of statistical assumptions in studies linking solar variability to climate, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19776, https://doi.org/10.5194/egusphere-egu26-19776, 2026.

EGU26-20122 | ECS | Posters on site | EOS4.4

Developing Matrix-Matched Empirical Calibrations for EDXRF Analysis of Peat-Alternative Growth Media 

Thulani De Silva, Carmela Tupaz, Maame Croffie, Karen Daly, Michael Gaffney, Michael Stock, and Eoghan Corbett

A key reason for the widespread use of peat-based growth media in horticulture is their reliable nutrient availability when supplemented with fertilisers. However, due to environmental concerns over continued peat-extraction and use, peat-alternatives (e.g., coir, wood fibre, composted bark, biochar) are increasingly being used commercially. These alternative media often blend multiple materials, making it crucial to understand elemental composition and nutrient interactions between components. This study evaluates whether benchtop Energy Dispersive X-ray Fluorescence (EDXRF) can provide a rapid method for determining the elemental composition of peat-alternative components.

Representative growing media components (peat, coir, wood fibre, composted bark, biochar, horticultural lime, perlite, slow-release fertilisers, and trace-element fertiliser) were blended in different ratios to generate industry-representative mixes. Individual components and prepared mixes were dried and milled to ≤80 μm. An industry-representative mix (QC-50: 50% peat, 30% wood fibre, 10% composted bark, 10% coir, with fertiliser and lime additions) and 100% peat were analysed by EDXRF (Rigaku NEX-CG) for P, K, Mg, Ca, S, Fe, Mn, Zn, Cu and Mo, and compared against ICP-OES reference measurements. The instrument’s fundamental parameters (FP) method using a plant-based organic materials library showed large discrepancies relative to ICP-OES (relative differences: 268–390 084%) for most elements in both QC-50 and peat, with the exception of Ca in QC-50 (11%). These results confirm that the FP approach combined with loose-powder preparation is unsuitable for accurate elemental analysis of organic growing media.

An empirical calibration was subsequently developed using 18 matrix-matched standards (CRMs, in-house growing media and individual component standards). Matrix matching is challenging because mixes are mostly organic by volume, yet variable inorganic amendments (e.g., lime, fertilisers, and sometimes perlite) can strongly influence XRF absorption/enhancement effects. Calibration performance was optimised iteratively using QC-50 as the validation sample, until relative differences were <15% for all elements. When applied to 100% peat, agreement with ICP-OES results improved substantially for some macro-elements (e.g. Mg 10%, Ca 1%, S 19%) but remained poor for most trace elements (28–96%), demonstrating limited transferability of this calibration method across different elements and matrices tested.

Overall, these results demonstrate that loose powder preparation does not provide sufficiently robust accuracy for EDXRF analysis of organic growing media even with meticulous empirical matrix-matched calibration. We are therefore developing a pressed pellet method using a low-cost wax binder to improve sample homogeneity (packing density) and calibration transferability. Twenty unknown mixes will be analysed using both loose powder and pressed-pellet calibrations, and agreement with reference data (ICP-OES) will confirm method validation, supporting the development of EDXRF as a novel approach for growing media analysis.

How to cite: De Silva, T., Tupaz, C., Croffie, M., Daly, K., Gaffney, M., Stock, M., and Corbett, E.: Developing Matrix-Matched Empirical Calibrations for EDXRF Analysis of Peat-Alternative Growth Media, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20122, https://doi.org/10.5194/egusphere-egu26-20122, 2026.

EGU26-20375 | ECS | Posters on site | EOS4.4

From Field to File: challenges and recommendations for handling hydrological data 

Karin Bremer, Maria Staudinger, Jan Seibert, and Ilja van Meerveld

In catchment hydrology, long-term data collection often starts as part of a (doctoral) research project. In some cases, the data collection continues on a limited budget, often using the field protocol and data management plan designed for the initial short-term project. Challenges and issues with the continued data collection are likely to arise, especially when there are multiple changes in the people involved. It is especially difficult for researchers who were not directly involved in the fieldwork to understand the data and must therefore rely on field notes and archived data. They then often encounter issues related to inconsistent metadata, such as inconsistent date-time formats and inconsistent or missing units, missing calibration files, and unclear file and processing script organization.

While the specific issues may sound very case-dependent, based on our own and other’s experiences from various research projects, it appears that many issues recur more frequently than one might expect (or be willing to admit). In this presentation, we will share our experiences with bringing spatially distributed groundwater level data collected in Sweden and Switzerland from the field to ready-to-use files. Additionally, we provide recommendations for overcoming the challenges during field data collection, data organization, documentation, and data processing using scripts. These include having a clear, detailed protocol for in the fieldwork and the data processing steps, and ensuring it is followed. Although protocols are often used, they are frequently not detailed enough or are not used as designed. The protocols might also not take into account the further use of the data, such as for hydrological modelling, beyond field collection. 

How to cite: Bremer, K., Staudinger, M., Seibert, J., and van Meerveld, I.: From Field to File: challenges and recommendations for handling hydrological data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20375, https://doi.org/10.5194/egusphere-egu26-20375, 2026.

In 2014 we developed the Wageningen Lowland Runoff Simulator (WALRUS), a conceptual rainfall-runoff model for catchments with shallow groundwater. Water managers and consultants were involved in model development. In addition, they sponsored the steps necessary for application: making an R package, user manual and tutorial, publishing these on GitHub and organising user days. WALRUS is now used operationally by several Dutch water authorities and for scientific studies in the Netherlands and abroad. When developing the model, we made certain design choices. Now, after twelve years of application in water management, science and education, we re-evaluate the consequences of those choices.

The lessons can be divided into things we learned about the model’s functioning and things we learned from how people use the model. Concerning the model’s functioning, we found that keeping the model representation close to reality has advantages and disadvantages. It makes it easy to understand what happens and why, but it also causes unrealistic expectations. Certain physically based relations hampered model performance because they contained thresholds, and deriving parameter values from field observations resulted in uncertainty and discussions about spatial representativeness.

Concerning the practical use, we found that the easy-to-use, open source R package with manual was indispensable for new users. Nearly all users preferred default options over the implemented user-defined functions to allow tailor-made solutions. Parameter calibration was more difficult than expected because the feedbacks necessary to simulate the hydrological processes in lowlands increase the risk of equifinality. In addition, lack of suitable discharge data for calibration prompted the request for default parameter values. Finally, the model was subject to unintended model use, sometimes violating basic assumptions and sometimes showing unique opportunities we had not thought of ourselves.

C.C. Brauer, A.J. Teuling, P.J.J.F. Torfs, R. Uijlenhoet (2014): The Wageningen Lowland Runoff Simulator (WALRUS): a lumped rainfall-runoff model for catchments with shallow groundwater, Geosci. Model Dev., 7, 2313-2332, doi:10.5194/gmd-7-2313-2014

How to cite: Brauer, C.: Re-evaluating the WALRUS rainfall-runoff model design after twelve years of application, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21915, https://doi.org/10.5194/egusphere-egu26-21915, 2026.

In the Lower Bavarian–Upper Austrian Molasse Basin, a regionally extensive and water-resources–relevant thermal groundwater system occurs within the Upper Jurassic carbonate rocks (Malm aquifer), extending from Regensburg to areas west of Linz. This resource has long been utilized on both sides of the national border for balneological purposes as medicinal and bathing water, as well as for geothermal energy production. It therefore represents a significant economic asset for the region and is of particular importance for regional water resource management.

Long-term monitoring and data obtained from pumping tests indicate hydraulic interference among some of these uses. To quantify and assess these interactions, a three-dimensional numerical model was developed and calibrated using observational data collected over several decades. The model will serve as a decision-support tool for future permitting processes, including new applications and modifications of existing uses.

Critical issues comprise the harmonization of heterogeneous datasets and the complex hydrothermal behavior of a steeply dipping aquifer, with localized geothermal gradient anomalies promoting thermally induced convection phenomena.The key innovations of the approach include full transient calibration of the whole reservoir over an analysis period of 100 years; consideration of thermal convection and density effects throuth uni-directional coupling;

Although the current application is restricted to geothermal systems, the modeling approach is methodologically transferable to other forms of subsurface utilization, such as carbon capture and storage (CCS), underground thermal energy storage (UTES), and related technologies as well as their interactions.

The results presented are based on a work under the commission of the Thermal Water Expert Group, acting on behalf of the Permanent Water Commission established under the Regensburg Treaty, and represented by the following institutions:
• Office of the Upper Austrian Provincial Government,
• Bavarian Environment Agency,
• Austrian Federal Ministry of Agriculture and Forestry.

The main publication is available for download (in German language) here: https://www.land-oberoesterreich.gv.at/files/publikationen/w_thermalwasser_bayern_ooe.pdf

How to cite: Hoyer, S., Bottig, M., and Schubert, G. and the ARGE Thermalwasser: Numerical modelling of a carstic aquifer body as decision support tool for deep geothermal applications and their interference. The transboundary upper jurassic carbonates as a case study., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5331, https://doi.org/10.5194/egusphere-egu26-5331, 2026.

Carbon capture and sequestration (CCS) is believed to play a critical role in achieving the European Union’s climate neutrality targets, particularly for emissions from hard-to-abate sectors. Recent policy developments in Austria, including renewed discussions on geological CO₂ storage and increased integration into the EU carbon market, have intensified interest in evaluating domestic CCS potential. The Vienna Basin represents Austria’s most promising onshore CCS candidate, owing to its extensive subsurface dataset, long production history, and proven performance as a storage province.

This study assesses the feasibility of CCS in the Vienna Basin with a specific focus on pressure-driven interactions between CO₂ injection and other subsurface operations. A basin-scale reservoir model is developed to represent the key stratigraphic units, structural elements, and hydraulic connections relevant for CO₂ storage. Using this model, multiple injection scenarios are simulated to evaluate pressure evolution, pressure propagation away from the injection site, and the resulting pressure footprints at the basin scale.

Rather than focusing solely on CO₂ plume migration, the analysis emphasizes pressure waves generated by CO₂ injection and their transmission through permeable formations and fault zones. These pressure perturbations may extend well beyond the immediate storage complex and potentially affect neighboring subsurface activities, including underground gas storage, geothermal energy exploitation, and prospective hydrogen storage sites. Scenario results are used to quantify the magnitude and spatial extent of pressure increases and to assess their implications for operational pressure limits, injectivity, and fault stability in adjacent reservoirs.

The results are synthesized into a feasibility framework that links geological suitability, pressure management, and multi-use compatibility. This framework provides guidance on favorable storage domains, critical constraints, and key uncertainties associated with CCS deployment in the Vienna Basin.

How to cite: Abdellatif, M. and Ott, H.: Evaluating Carbon Capture and Storage Feasibility in the Vienna Basin: Pressure Propagation, Formation Integrity, and Multi-Use Subsurface Impacts, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6712, https://doi.org/10.5194/egusphere-egu26-6712, 2026.

EGU26-8850 | ECS | Orals | ERE6.2

Pore-scale formation of CO₂ hydrates in sandstone and global assessment of hydrate-based CO₂ storage potential in marine sediments 

Xiuping Zhong, Wei Guo, Praveen Linga, Pengyu Zhang, Chen Chen, and Xiaochu Wang

Hydrate-based geological storage of CO₂ is a solid-state CCUS technology characterized by high thermodynamic stability and long-term safety, and  is therefore regarded as a promising pathway for large-scale CO₂ sequestration. Sandstone formations widely distributed in marine sediments provide substantial pore volume and are considered favorable targets for CO₂ storage. In this study, the pore-scale formation behavior of CO₂ hydrates in sandstone was systematically investigated, and the global CO₂ storage potential in marine sandstones was further assessed.

In the first part of this work, sandstone pore structures were characterized using thin-section petrography, mercury intrusion porosimetry (MIP), and nuclear magnetic resonance (NMR) measurements. The NMR-derived pore size distribution was calibrated against the MIP results, showing excellent agreement (R² = 99.5%) and indicating that the pore sizes of the tested sandstone mainly ranged from 0.005 to 500 μm. Subsequently, in situ CO₂ hydrate formation experiments were conducted using an NMR-based hydrate formation and monitoring system at temperatures of 1–7 °C and pressures of 2–8 MPa, revealing both the kinetic and thermodynamic characteristics of CO₂ hydrate formation in micro- and nanopores. In the second part, global standard datasets were employed to estimate the volume of marine sedimentary sandstones suitable for hydrate-based CO₂ storage, and these results were combined with the water-to-hydrate conversion ratios obtained from laboratory experiments to quantify the total amount of CO₂ that could be stored in marine sediments.

The results indicate that due to the combined effects of pore confinement and the Kelvin effect, the equilibrium pressure of CO₂ hydrates at 7 °C in pores with a pore diameter of approximately 10 nm is elevated from about 2.87 MPa under bulk conditions to 6–8 MPa. When pore sizes exceed 0.1 μm, the influence of pore size on hydrate formation efficiency becomes negligible. Moreover, the large specific surface area provided by rock pores (2.186 m²/g for the samples used in this study) substantially reduces the nucleation energy barrier, leading to rapid hydrate formation kinetics, with all experimental groups reaching approximately 90% of the final conversion within 140 min. Under the investigated pressure–temperature conditions, the water-to-hydrate conversion ratio in pores larger than 0.1 μm ranges from 0.35 to 0.85.

Global-scale estimation suggests that the effective volume of marine sediments suitable for CO₂ hydrate formation within water depths shallower than 4000 m is approximately 3.48 × 10¹⁵ m³. Assuming a sandstone fraction of 1%, the corresponding theoretical CO₂ storage capacity reaches about 1324 Gt, which is close to half of the cumulative anthropogenic CO₂ emissions since the Industrial Revolution. This study provides strong scientific support for large-scale and safe geological sequestration of CO₂ and offers a potential technological pathway toward achieving global carbon neutrality.

How to cite: Zhong, X., Guo, W., Linga, P., Zhang, P., Chen, C., and Wang, X.: Pore-scale formation of CO₂ hydrates in sandstone and global assessment of hydrate-based CO₂ storage potential in marine sediments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8850, https://doi.org/10.5194/egusphere-egu26-8850, 2026.

EGU26-9250 | ECS | Posters on site | ERE6.2

How the “One County, One Product” model reshapes regional ecological vulnerability : Evidence from Shunping county 

Jianwei Li, Hongjun Liu, Wei Wan, Shiwen Liu, and Zhong Liu

Most existing studies on ecological vulnerability assessment focus on large-scale regions, which limits their ability to accurately capture the ecological specificity and underlying driving mechanisms of small-scale areas. Small-scale ecosystems, such as those at the county level, often exhibit pronounced regional characteristics. Their natural endowments, industrial structures, and socio-cultural factors not only shape local ecological conditions but also play an important role in the sustainable development of surrounding areas. Consequently, there is an urgent need for targeted research on such regions and for the formulation of corresponding management strategies.

Taking Shunping County as a case study, this research extends the traditional SRP (Sensitivity–Resilience–Pressure) framework by introducing a “Characteristic” dimension and develops a CSRP (Characteristic–Sensitivity–Resilience–Pressure) model. By integrating the Analytic Hierarchy Process (AHP) and the entropy weight method, the ecological vulnerability of Shunping County was quantitatively evaluated. The spatiotemporal evolution patterns and driving factors were further analyzed, and corresponding management strategies were proposed.

The results indicate that ecological vulnerability in Shunping County exhibited a “deterioration followed by improvement” trend in 2010, 2015, and 2020. These changes were influenced not only by natural factors but also closely associated with the implementation of local policies. Spatially, ecological vulnerability was relatively high in the southeastern plain areas due to intensive human activities and pollution from characteristic industries, whereas the northwestern mountainous and hilly areas showed comparatively lower vulnerability. The driving factor analysis reveals that the interactive effects of socioeconomic development, industrial structure, and population distribution exert a stronger influence on ecological vulnerability than any single natural factor. In addition, pollution control related to industrial activities remains a key issue requiring particular attention in the region.

The findings provide both theoretical and practical implications for ecological management and sustainable development in Shunping County. The proposed CSRP model offers a transferable analytical framework for assessing ecological vulnerability in small-scale regions with distinct local development characteristics. It is particularly useful for understanding socio-ecological interactions in urban areas and their surroundings under environmental pressures and adaptive governance processes, and it can serve as a reference for monitoring, assessment, and sustainable strategy design in the context of urban–rural coordinated transformation.

How to cite: Li, J., Liu, H., Wan, W., Liu, S., and Liu, Z.: How the “One County, One Product” model reshapes regional ecological vulnerability : Evidence from Shunping county, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9250, https://doi.org/10.5194/egusphere-egu26-9250, 2026.

EGU26-10035 | Posters on site | ERE6.2

Systemic blue-green-red urban development (URBAN LE) – A Helmholtz Solution Lab 

Jan Friesen, Uwe Hampel, Katharina Schaufler, Daniel Lang, Lucie Moeller, Magdalena Scheck-Wenderoth, Hannes Hofmann, Fabian Brandenburg, and Roland Müller

The URBAN LE project advances climate-resilient urban development by establishing an integrated blue-green-red (BGR) infrastructure framework that reinforces water security and supports sustainable urban transformation. Based in Leipzig and involving five Helmholtz Centers (UFZ, HZDR, HIOH/HZI, GFZ, and KIT), it integrates inter- and transdisciplinary research with co-designed implementation alongside the City of Leipzig and a broad network of municipal, national, and international cities. URBAN LE addresses stormwater management, water-energy coupling, water quality, and governance innovation through real-world pilot implementations at the UFZ campus, and at different sites throughout city. Using functional digital twins and co-designed planning tools, the project evaluates scalable solutions for reducing potable water demand, enhancing water retention and treatment, and integrating aquifer thermal energy storage (ATES). A central focus is the identification of chemical and microbial pollutants mobilized during extreme weather events, including their quantification, accumulation, fate, and transport within BGR systems. Functional digital twins enable comprehensive urban system analysis by combining numerical modeling of hydrological and hydrothermal processes, scenario integration of climatic, demographic, and economic drivers, and infrastructure planning and optimization—such as evaluating interactions between irrigation methods and thermal networks in sponge-city scenarios.

URBAN LE contributes to “Urban Blue-Green-Red Water Systems” and tackles challenges such as decentralized infrastructure planning, digitalization, and institutional governance. Its systemic design positions Leipzig as a model city and facilitates replication in at least ten further German and European cities. By merging rigorous scientific innovation with municipal co-creation, URBAN LE delivers robust tools for climate adaptation, energy transition, and urban water reuse, ensuring long-term impact.

How to cite: Friesen, J., Hampel, U., Schaufler, K., Lang, D., Moeller, L., Scheck-Wenderoth, M., Hofmann, H., Brandenburg, F., and Müller, R.: Systemic blue-green-red urban development (URBAN LE) – A Helmholtz Solution Lab, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10035, https://doi.org/10.5194/egusphere-egu26-10035, 2026.

EGU26-10966 | ECS | Orals | ERE6.2

Potential of CO2 storage opportunities and the role of natural CO2 reservoirs in the Pannonian Basin 

Dóra Cseresznyés, Csilla Király, Ágnes Szamosfalvi, Zsuzsanna Szabó-Krausz, Csaba Szabó, and György Falus

One of the key elements to achieve a low-carbon and sustainable future is to utilize the porous media in the subsurface. Carbon dioxide capture, utilization and storage is a promising way to use the subsurface and reduce anthropogenic greenhouse gas emissions, especially carbon dioxide. The Pannonian Basin, shared by Central-Eastern European countries, is one of the most prospective areas of onshore CO2 geological storage in Europe. Late Miocene sedimentary rocks of the Pannonian Basin offer significant potential for storing large gas volumes. Storage potential assessment focused on two major groups of geological structures: depleted hydrocarbon reservoirs and saline aquifers. The CO2 storage capacity of the potential fields was estimated based on volumetric parameters. The total CO2 storage capacity of the depleted hydrocarbon fields is estimated to be ~97 Mt whereas in deep saline reservoirs is estimated to fall ~760 Mt. The reservoir rock with the highest storage potential consists of turbiditic sandstone, which is widespread and has regional extent in the Pannonian Basin.
The mechanisms of storage and the effect of CO2 on porous rock still raises questions. Natural CO2 occurrences have developed in similar geological structures to hydrocarbon reservoirs and represent a unique opportunity to study and understand the long-term fate of CO2 in reservoir structures. Core samples from natural CO2 reservoirs were investigated by detailed modal, textural and geochemical analysis. With isotope geochemistry (stable C, O and H isotopes in carbonates) and geochemical modeling (with PHREEQC) tools, we aim to shed light on which carbonates precipitated as a response to CO2 flooding, and to estimate the mineral interactions on geological time scale (Falus et al., 2025).

How to cite: Cseresznyés, D., Király, C., Szamosfalvi, Á., Szabó-Krausz, Z., Szabó, C., and Falus, G.: Potential of CO2 storage opportunities and the role of natural CO2 reservoirs in the Pannonian Basin, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10966, https://doi.org/10.5194/egusphere-egu26-10966, 2026.

EGU26-12313 | Posters on site | ERE6.2

Challenges and opportunities for the multi-use of geothermal resources in urban areas 

Paweł Wojnarowski, Leszek Pająk, Barbara Tomaszewska, Michał Kaczmarczyk, and Damian Janiga

Decarbonising district heating systems poses a significant challenge in Central and Eastern Europe, as high-temperature networks predominantly rely on coal-fired power stations. State policy has expanded the number of sites, facilitating the exploration and development of geothermal energy resources while prioritising subsidies for drilling new wells in regions with intermediate geological exploration. A rise in new activity pertaining to the exploration and development of geothermal resources has been observed. One of such locations is Konin in central Poland. However, exploring geothermal resources in urban environments is hindered by limited data availability, dense infrastructure, and legal constraints. Access may also be restricted and constrained by open spaces and road accessibility. Conventional geothermal evaluations in Polish cases predominantly rely on well-drilling data, geophysical surveys, and thermal-gradient measurements. In addition, most geothermal systems utilise saline geothermal fluids as the energy carrier. Regrettably, most geothermal systems face several technological challenges associated with the disposal of saline geothermal fluids. In the presented work, the limitations of available data are analysed, and the necessity of advanced exploration methods, such as seismic surveys, is highlighted for the Konin site as a case study. To facilitate the development of the geothermal system, seismic surveys tailored to the urban area's specific characteristics have been planned. The surveys are being carried out as part of the URGENT project, which aims to provide sustainable and affordable solutions for urban seismic exploration of geothermal resources. Alternative methods of obtaining geothermal energy are also indicated in this case, thereby limiting problems related to high water mineralisation and enabling closed-loop systems, evaluated as part of the HOCLOOP project. In this configuration, the system can also be used for underground surplus energy storage, enabling wider use of underground structures. The results highlight the essential importance of data integrity and completeness in reducing investment risks and enhancing geothermal resource utilisation. They point to the importance of a comprehensive approach to the use of geothermal resources in urban areas. The application of such a solution enables a rational transition from coal-based heating systems to low-emission systems and multi-use of the subsurface structures.

How to cite: Wojnarowski, P., Pająk, L., Tomaszewska, B., Kaczmarczyk, M., and Janiga, D.: Challenges and opportunities for the multi-use of geothermal resources in urban areas, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12313, https://doi.org/10.5194/egusphere-egu26-12313, 2026.

EGU26-13055 | Orals | ERE6.2

Geothermal-lithium co-production from subsurface brines: comparing technological and policy pathways across the Leduc Formation (Canada) and the Buntsandstein (Germany/France) 

Amin Ghanizadeh, Ahmed Elmeligy, Katherine Westerlund, Najmeh Khaleghifar, Nilesh P. Joisar, Adnan Younis, Afshin Ghanizadeh, Hamidreza Hamdi, Christopher R. Clarkson, Katrin Brömme, Timo M. König, Christoph König, David Eaton, Benjamin Tutolo, Per K. Pedersen, Natasha Morris, and Kirsten Pugh

Co-producing geothermal energy and critical elements (notably lithium, Li) from deep subsurface brines is emerging as a “two-for-one” subsurface use[1,2]: renewable heat/power plus domestic supply of battery materials. Yet, the feasibility of geothermal-Li co-development is shaped by coupled constraints spanning reservoir deliverability, fluid chemistry, process integration, and permitting regimes[3,4]. Here we compare technological and policy designs of geothermal-Li co-development using two representative deep saline aquifer systems: (1) the Devonian Leduc Formation in the Western Canadian Sedimentary Basin (Alberta, Canada), and (2) the Triassic Buntsandstein (Bunter Sandstone) reservoirs of the Upper Rhine Graben (Germany/France).

For the Leduc Formation, we expand on our prior feasibility work[1,2] focused on deep (>1.5 km) aquifers and regulatory pathways that already combine geothermal development and brine-hosted mineral considerations within Alberta’s existing energy and injection governance (e.g., Directives 089 and 090). A Python-based, multi-criteria geospatial screening analysis[1] integrated temperature, Li occurrence, geologic constraints, proximity to recorded seismicity, and Indigenous rights-holder considerations to narrow to a preferred candidate locality near Whitecourt/Fox Creek region. This quantitative screening analysis first targeted areas where modeled subsurface temperatures exceed 100 °C and then intersected these “hot spots” with formation-water datasets indicating elevated dissolved Li, through a basin-scale mapping approach[2]. Among the candidate areas, there were regions that fall within multiple Indigenous territories (e.g., Treaty 6 and 8), located within 10s km radius of nearby First Nations reserves (e.g., Alexander 134A), highlighting stakeholder engagement as an operational constraint alongside technical screening.

For the Buntsandstein of the Upper Rhine Graben (Germany/France), we build on existing works, targeting deep (~2.5–5 km) Triassic sandstone reservoirs[5]. Published datasets indicate geothermal brines with Li concentrations in the ~160–200 mg/L range, hosted in settings where the Buntsandstein can form a principal reservoir unit[6,7]. Lithium enrichment is linked to a complex hydrothermal history and interaction with sedimentary and evaporitic components of the rift fill, implying that resource sustainability cannot be inferred from “static” brine grades alone. Recent reservoir-scale modeling based on Upper Rhine Graben stratigraphy indicates that, under plausible reinjection–production connectivity, Li concentrations may decline over multi-decadal operation (order-tens of percent), even while heat production remains comparatively stable, making flow rate, reinjection strategy, and extraction efficiency the dominant levers for long-run performance[5,7]. On the German side, this co-development is governed through state mining authorities by issuing exploration titles explicitly covering “Erdwärme, Sole und Lithium” under the Federal Mining Act (BBergG)[8,9], with project execution governed parallel with water-law permissions for brine handling/reinjection.

Across both regions, we identify a practical policy design lesson: geothermal-li projects would benefit under integrated regulation as “closed-loop” subsurface systems, with adaptive monitoring triggers tied to (a) reservoir pressure, (b) reinjection breakthrough and Li decline trajectories, and (c) scaling/corrosion and waste streams from direct lithium extraction process. By aligning and comparing subsurface governance with coupled thermo-hydro-chemical characteristics of these resources globally, regulators can better capture synergies (energy + minerals) while containing shared risks, accelerating responsible deployment in both mature hydrocarbon basins and geothermal provinces.

How to cite: Ghanizadeh, A., Elmeligy, A., Westerlund, K., Khaleghifar, N., Joisar, N. P., Younis, A., Ghanizadeh, A., Hamdi, H., Clarkson, C. R., Brömme, K., König, T. M., König, C., Eaton, D., Tutolo, B., Pedersen, P. K., Morris, N., and Pugh, K.: Geothermal-lithium co-production from subsurface brines: comparing technological and policy pathways across the Leduc Formation (Canada) and the Buntsandstein (Germany/France), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13055, https://doi.org/10.5194/egusphere-egu26-13055, 2026.

EGU26-13739 | Orals | ERE6.2

Venice and its lagoon under sea-level rise: transformative choices for a coastal socio-ecological system 

Piero Lionello, Valeria Di Fant, Ulysse Pasquier, Luigi Tosi, Le Cozannet Goneri, Robert J. Nicholls, Wolfgang Cramer, Roger Cremades Rodeja, Carlo Giupponi, Jochen Hinkel, Adriano Sfriso, Athanasios T. Vafeidis, Georg Umgiesser, and Marjolijn Haasnoot

Venice and its lagoon form a tightly coupled coastal socio-ecological system in which urban fabric, cultural heritage, lagoon ecosystems and regional infrastructures jointly determine vulnerability and resilience to sea-level rise. As relative sea level continues to increase due to climate change and subsidence, adaptation in Venice cannot be limited to incremental risk reduction but requires transitions between fundamentally different strategies.

This contribution applies an adaptation pathways perspective to the Venice–lagoon system to examine how the available solution space decreases under rising sea level. Four adaptation strategies are considered: an open-lagoon configuration based on mobile barriers and accommodation measures, ring-diking that isolates the historic city and other settlements from the lagoon, (closed-lagoon configuration with permanent coastal barriers), and retreat through relocation or abandonment. The  analysis focuses on how physical constraints, ecological impacts, social acceptability and long lead times interact to shape transitions between these strategies as sea level rise continues.

The Venice case illustrates how climate and geo-processes, infrastructures, available technical solutions  and cultural values condition the timing and characteristics of adaptation tipping points, beyond which strategies can no longer meet their intended goals. By explicitly linking alternative strategies to distinct socio-ecological transformations of the city and its surrounding environment, the pathways approach helps clarify trade-offs, irreversibilities and decision time windows for urban transformation under deep uncertainty.

The results highlight the importance of early, anticipatory planning for coastal cities facing long-term sea-level rise, and demonstrate how geoscience-informed adaptation pathways can support governance of transformative change in complex urban regions.

 

 

How to cite: Lionello, P., Di Fant, V., Pasquier, U., Tosi, L., Goneri, L. C., Nicholls, R. J., Cramer, W., Cremades Rodeja, R., Giupponi, C., Hinkel, J., Sfriso, A., T. Vafeidis, A., Umgiesser, G., and Haasnoot, M.: Venice and its lagoon under sea-level rise: transformative choices for a coastal socio-ecological system, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13739, https://doi.org/10.5194/egusphere-egu26-13739, 2026.

EGU26-13999 | Orals | ERE6.2

Leveraging  Synergies: From Fragmented Development to Integrated Underground Planning 

Katrin Pakizer and Fabienne Sierro

The subsurface represents a critical frontier for achieving sustainability goals, yet current development approaches remain largely uncoordinated and reactive. As societal challenges intensify —from climate change mitigation to urban densification— the underground is increasingly recognized as essential infrastructure space. However, the prevailing "first-come, first-served" or "last-resort" principles governing subsurface allocation result in fragmented management practices that overlook valuable synergistic opportunities between different underground uses. The question therefore arises how subsurface synergies can be strategically integrated into regulation and planning frameworks to promote sustainable, long-term underground development.

We identify three core principles that enable effective subsurface synergies: multifunctionality, circularity, and repurposing. Multifunctionality recognizes that underground spaces can serve multiple purposes simultaneously or sequentially, such as combining geothermal energy extraction with thermal energy storage, or integrating transport infrastructure with utility corridors. Circularity emphasizes cascading energy uses and resource efficiency, exemplified by utilizing waste heat from data centers for district heating networks or repurposing abandoned mines for energy storage. Repurposing extends the lifecycle of underground investments by adapting existing infrastructure to new functions, thereby reducing environmental impacts and optimizing resource utilization.

Through real-world case studies, we demonstrate how these principles can be operationalized within master planning and regulatory frameworks. These cases reveal both the opportunities for synergistic subsurface planning and the governance challenges that emerge from competing uses, jurisdictional fragmentation, and temporal mismatches between planning horizons and underground resource dynamics. Moreover, our analysis highlights critical barriers to achieving subsurface synergies: inadequate legal frameworks that fail to recognize three-dimensional property rights and long-term resource claims; sectoral silos separating energy, water, infrastructure, and environmental governance; insufficient data sharing and transparency about existing and planned underground uses; and lack of coordination mechanisms between stakeholders with different temporal perspectives and priorities. Overcoming these barriers requires moving beyond conflict resolution toward proactive synergy identification and facilitation.

We propose that effective subsurface governance must adopt a holistic, interdisciplinary, and integrated approach combining technical assessment with policy innovation. This includes developing spatial planning tools that visualize underground uses across multiple dimensions; establishing coordination platforms that bring together geoscientists, engineers, policymakers, and affected communities; creating legal mechanisms that recognize and incentivize synergistic developments; and implementing monitoring frameworks that track interactions between subsurface uses over time.

Our presentation contributes to the session's objectives by demonstrating how governance frameworks can either enable or constrain subsurface synergies, and by providing practical insights for researchers, policymakers, and practitioners seeking to leverage underground resources more sustainably. As pressure on subsurface space intensifies, the ability to identify, evaluate, and implement synergistic solutions becomes essential for ensuring that underground development serves both current and future societal needs while respecting environmental limits and intergenerational equity.

 

How to cite: Pakizer, K. and Sierro, F.: Leveraging  Synergies: From Fragmented Development to Integrated Underground Planning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13999, https://doi.org/10.5194/egusphere-egu26-13999, 2026.

EGU26-14432 | Orals | ERE6.2 | Highlight

Decarbonizing cities from below: deep geothermal energy as a pillar of urban transformation 

Sven Fuchs, Guido Blöcher, Ben Norden, Cornelia Schmidt-Hattenberger, Erik Spangenberg, Simona Regenspurg, Hannes Hofmann, Stefan Kranz, Harald Milsch, and Ingo Sass

Cities are hubs of resource consumption and hotspots of vulnerability, yet they are also places where climate-neutral solutions need be co-designed, tested, and scaled. A central gap in many transformation pathways is that urban energy strategies are still planned largely “from the surface”, while the subsurface and its capacities and constraints remains underexplored in socio-technical and governance-oriented transformation research. This talk positions the subsurface as a core element of integrated urban energy infrastructure within the blue–green–red framing: ensuring groundwater and water quality (blue), and shaping land-use, nature-based solutions (green) interacting with low-carbon heat and power supply (red). We focus on geothermal heat as a practical, scalable option for decarbonizing urban heat supply, while it is reducing exposure to volatile fuel imports and supporting resilient district heating concepts. With a specific subsurface focus using Potsdam as an illustrative case, we outline what it takes to make geothermal a planning-ready solution. The key message is that the subsurface is not only a boundary condition but an indispensable factor and an enabling infrastructure layer for climate-neutral urban transformation. Bringing it systematically into planning and governance is essential for robust mitigation and adaptation strategies that meet cities’ sustainability and resilience targets.

How to cite: Fuchs, S., Blöcher, G., Norden, B., Schmidt-Hattenberger, C., Spangenberg, E., Regenspurg, S., Hofmann, H., Kranz, S., Milsch, H., and Sass, I.: Decarbonizing cities from below: deep geothermal energy as a pillar of urban transformation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14432, https://doi.org/10.5194/egusphere-egu26-14432, 2026.

EGU26-14910 | ECS | Posters on site | ERE6.2

Reverse Engineering for the Chronology of Medieval Aqueducts: A Case Study of the Holy Monastery of Dochiariou, Mount Athos 

Nikolaos Papadodimas, Georgios David Laoutaris, Nikos Mamassis, and G.-Fivos Sargentis

Although extensive information exists on the chronological evolution of the fortified monastic complexes on Mount Athos, data regarding the construction dates of their hydraulic infrastructure remain comparatively limited. Since water constitutes a fundamental prerequisite for sustained settlement and construction, the development of a monastery presupposes access to reliable and sufficient natural resources essential for its establishment and long-term survival. This study applies a quantitative reverse-engineering approach to estimate the water demands associated with the construction of Dochiariou Monastery's principal fortified elements, namely the katholikon, the tower , and the perimeter walls. By approximating the number of monks, draught animals , and construction workforce, as well as the volumes of building materials (brick, stone , and lime mortar), we quantify minimum water requirements for mortar production, brick making, human and animal consumption, and material transport along the steep kalderimi (stone-paved path) from the Αrsanas (dock). Order-of-magnitude calculations indicate that the annual water yield of local springs  provides only a marginal surplus, insufficient to sustain intensive, multi-year construction phases in the absence of engineered storage or supplementary water sources. The central aqueduct—terminating directly into the tower—exhibits a high potential discharge capacity and a strategically integrated layout, suggesting that it may have predated the major building campaigns. This analysis indicates that the aqueduct and associated hydraulic works were likely among the earliest infrastructural interventions, enabling subsequent expansion in an isolated, topographically constrained environment. The findings demonstrate the value of reverse engineering as a methodological tool for inferring the relative chronology and functional role of medieval hydraulic systems, particularly where direct archaeological or archival evidence is scarce. These insights further underscore adaptive water-management strategies that underpin long-term settlement resilience in resource-limited environments.

How to cite: Papadodimas, N., Laoutaris, G. D., Mamassis, N., and Sargentis, G.-F.: Reverse Engineering for the Chronology of Medieval Aqueducts: A Case Study of the Holy Monastery of Dochiariou, Mount Athos, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14910, https://doi.org/10.5194/egusphere-egu26-14910, 2026.

To quantitatively assess the increasingly severe light pollution in recent years, approaches capable of estimating night sky brightness with high spatial-temporal precision is crucial. However, Falchi et al. (2016) global model did not adequately represent variations in environmental conditions such as aerosols. Therefore, this study developed a new regional-scale night sky brightness model capable of accounting for local characteristics.

This model inputs aerosol, ground-based artificial light, and surface reflectance, and performs radiative transfer calculations that consider multiple scattering in the atmosphere and multiple reflections at the surface. Furthermore, it considers a point spread function based on the Monte Carlo method and calculates the night sky brightness as a hemispherical mean radiance.

The results enabled a better reproduction of the spatial distribution of brightness in urban areas and provided estimates closer to observed values in Japan compared to Falchi et al. (2016).

Fig. 1 The areas and their distribution of night sky brightness, calculated for seven urban areas in Japan.

Additionally, analysis of long-term variations in seven large cities in Japan using this model suggests that night sky brightness generally correlates with population size while also being influenced by urban structure. Although no significant increasing trend was observed between 2013 and 2023, brightness decreased in many cities during the COVID-19 pandemic period, with contributions from both ground-based artificial light and aerosol changes indicated.

This study provides a new assessment methodology, applicable not only within Japan but also extendable to regions worldwide, for quantitatively understanding the current state and variation factors of light pollution.

How to cite: Sano, M. and Iwabuchi, H.: Reproduction of night sky brightness variations in urban areas of Japan caused by aerosols, artificial ground-based light, and surface reflectance, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15384, https://doi.org/10.5194/egusphere-egu26-15384, 2026.

EGU26-15773 | ECS | Orals | ERE6.2

Decoding Socio-Ecological Dynamics for Urban Resilience: A 30-Year Study of Ecosystem Health and Its Drivers in the Guanzhong–Tianshui Economic Zone, China 

Wenjie Xiao, Wen Fan, Ya-ni Wei, Luke Kelleher, Weina Yuan, Shenyuan Zheng, and Zihao Shi

Densely populated urban regions are dual focal points of vulnerability and innovation, where socio-ecological dynamics fundamentally shape regional resilience to global environmental transformation. To decipher this dynamic process, this study adopts ecosystem health (EH) as the core lens to conduct a 30-year (1990–2020) empirical analysis of China's Guanzhong–Tianshui Economic Zone (GTEZ) — a region serving as both a key corridor of the Belt and Road Initiative and a typical area of urban expansion. Its spatial structure, bordered by the ecologically sensitive Loess Plateau to the north, sheltered by the Qinling Mountains ecological barrier to the south, and containing the densely populated Guanzhong Plain in the center, makes it an ideal case for investigating the response mechanisms of human-environment systems. The study period spans three critical transformative phases: rapid industrialization, the gradual establishment of an environmental regulatory framework, and the widespread awakening of ecological conservation awareness.

This research integrates multi-source remote sensing and statistical data within a “Vigor–Organization–Elasticity–Services” assessment framework to systematically characterize the spatiotemporal evolution of EH. It further synthesizes natural drivers (temperature, precipitation, downward longwave radiation) and anthropogenic drivers (PM₂.₅, population density) to reveal the underlying mechanisms. By comparing multiple machine learning models, the CatBoost model with superior performance was selected and combined with the SHAP method for attribution analysis. The main findings are: (1) EH changes followed a clear “deterioration-to-improvement” trajectory. The initial decline was linked to rapid industrialization and a lack of ecological protection, while subsequent improvement benefited from the refinement of environmental regulations and increased public ecological awareness. (2) The dominant drivers shifted significantly from socio-economic factors to natural factors, indicating that after initial containment of anthropogenic pressures, the influence of natural processes like climate change on regional environmental health has become increasingly prominent. (3) EH exhibited significant spatial heterogeneity, with high-value areas consistently distributed in the southern ecological barrier zone, while low-value areas were concentrated in the western and central basin regions, reflecting a spatial gradient of human disturbance intensity.

By employing explainable artificial intelligence methods, this study deepens the understanding of the dynamics within complex urban socio-ecological systems and provides a methodological reference for related monitoring and modeling research. The results not only offer a scientific basis for climate-adaptive spatial planning and ecological risk management in similar urbanizing regions but also help identify key intervention points for resilience building. Ultimately, this research provides empirical insights into how cities and their surrounding areas can proactively adapt to and shape sustainable socio-environmental transformation pathways through collaborative governance and systematic planning. It contributes to translating global sustainable development goals into localized, actionable implementation strategies and offers context-specific guidance for coordinating development and conservation in comparable regions.

How to cite: Xiao, W., Fan, W., Wei, Y., Kelleher, L., Yuan, W., Zheng, S., and Shi, Z.: Decoding Socio-Ecological Dynamics for Urban Resilience: A 30-Year Study of Ecosystem Health and Its Drivers in the Guanzhong–Tianshui Economic Zone, China, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15773, https://doi.org/10.5194/egusphere-egu26-15773, 2026.

EGU26-16068 | ECS | Posters on site | ERE6.2

Evaluating Pathways and Feasibility of District-Scale Building Decarbonization: A Municipal Case Study in Seoul 

SangMin Jeong, Yohan Choi, and Chan Park

Achieving national carbon neutrality requires actionable implementation at the municipal level. In Seoul's Dongdaemun-gu, buildings account for 65.2% of greenhouse gas emissions (998 ktCO₂eq, 2018) with ambitious reduction targets of 34% by 2030, 44.3% by 2034, and net-zero by 2050. However, most urban energy studies focus on individual buildings or employ national-level statistics, leaving a critical gap at the district (Gu) scale—where policy authority, infrastructure planning, and technical feasibility converge. This study addresses two key questions: which decarbonization pathway is more viable for district-scale implementation, and can these municipal targets be technically and economically achieved?

We employ City Energy Analyst (CEA) to simulate district-wide building energy systems for all buildings in Dongdaemun-gu. The model encompasses building thermal performance, heating and cooling systems, occupancy patterns, and district energy infrastructure, calibrated against national energy statistics and actual public building consumption data. We compare four scenarios: Current Policy (S0), Heat Pump Electrification Pathway (S1), District Energy & Fuel Cell Pathway (S2), and Integrated Net-Zero Pathway (S3). For each scenario, we quantify final energy consumption, direct building-sector emissions while separating grid decarbonization effects, and economic costs to identify the most feasible route to meeting municipal targets.

By conducting Urban Building Energy Modeling at the district administrative scale, this research bridges the gap between theoretical decarbonization scenarios and implementable municipal climate policies. The findings will quantify the trade-offs between distributed electrification and centralized geoenergy infrastructure, providing evidence-based guidance for how local governments can translate national carbon neutrality commitments into concrete technology deployment strategies. This approach demonstrates the critical role of district-scale analysis in advancing urban energy transformation and climate policy implementation.

This research was supported by Carbon Neutrality Specialized Graduate Program through the Korea Environmental Industry & Technology Institute(KEITI) funded by the Ministry of Climate, Energy and Environment(MCEE).

How to cite: Jeong, S., Choi, Y., and Park, C.: Evaluating Pathways and Feasibility of District-Scale Building Decarbonization: A Municipal Case Study in Seoul, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16068, https://doi.org/10.5194/egusphere-egu26-16068, 2026.

Urban rainwater represents a realistic but often simplified exposure pathway for cement-based construction materials used in small-scale urban infrastructure. In this study, we investigated the time-dependent interaction between natural rainwater and cementitious materials, focusing on pH evolution, CO₂-related processes, and elemental mobility in both normative mortars and systems incorporating incinerated sewage sludge ash (ISSA). Rainwater collected in Kraków (southern Poland) exhibits near-neutral pH values that decrease slightly with storage time, reflecting equilibration with atmospheric CO₂ and the absence of strong acidic inputs, consistent with buffering from alkaline, potentially carbonate-bearing, urban aerosols.

Leaching experiments conducted over 1, 3, and 6 months show systematically higher pH values in leachates compared to the original rainwater, reaching approximately 8.1–8.4 after one month and gradually decreasing toward near-neutral values (≈ 7.0–7.3) after six months. These pH variations demonstrate effective alkalinity buffering by the cementitious matrix, dominated at early stages by portlandite dissolution and alkali release. With increasing exposure time, leachate pH shifts toward that of the incoming rainwater. 

Mortars containing ISSA exhibit pH trends comparable to those of conventional systems, with slightly moderated alkalinity release, suggesting the influence of additional aluminosilicate, phosphate, and iron-bearing components on the overall buffering capacity of the composite matrix. The observed pH evolution and associated changes in elemental mobility are linked to early alkalinity buffering, intermediate carbonation, and long-term diffusion-controlled stabilization. Throughout the exposure period, near-neutral to mildly alkaline pH conditions suppress the solubility of trace elements and promote sorption and encapsulation mechanisms, with no evidence of delayed contaminant release.

The results indicated that under realistic urban rainwater conditions, both conventional and ISSA-containing cementitious materials maintain chemical stability and environmental compatibility. Therefore, it is essential to consider natural rainwater chemistry and time-dependent pH evolution when evaluating the long-term durability and environmental safety of small-scale infrastructure. In addition, ISSA, when incorporated into cementitious matrices in appropriate proportions, does not represent a secondary source of contamination and may be valorized as a construction additive rather than disposed of in landfills

Acknowledgment: The research for this publication has been supported by the budget of the Anthropocene Priority Research Area (Earth System Science Core Facility Flagship Project) under the Strategic Programme Excellence Initiative at Jagiellonian University

 

How to cite: Kasina, M., Wierzbicki, A., and Popów, W.: Rainwater interactions with ISSA-modified mortars: pH evolution, CO₂ buffering and implications for urban infrastructure and waste valorization, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16808, https://doi.org/10.5194/egusphere-egu26-16808, 2026.

EGU26-17873 | Orals | ERE6.2

Is there a Gap Between Promise and Practice? A Critical Assessment of Digital Twins for Sustainable and Resilient Smart Cities  

Silke Niehoff, Grischa Beier, Malte Reißig, and Stefanie Kunkel

Urban areas face intensifying socio-ecological and socio-technical challenges – from climate change impacts and resource depletion to increasing polarization – demanding innovative approaches to build societal resilience. Digital twins (DTs) are touted as transformative tools for urban management, promising enhanced monitoring and modelling to ultimately make cities more sustainable and adaptable (Patel et al., 2024; Silva et al., 2018). However, Helbing and Sánchez-Vaquerizo (2023) highlight potential controversies relating to the limitations of DTs in complex dynamical systems and the ethical implications of treating society as something to be managed and optimised (Helbing and Sánchez-Vaquerizo, 2023). Although the concept of DTs is frequently employed to integrate and analyse various data streams, simulate complex urban processes, and facilitate informed decision-making regarding climate change strategies, their actual deployment appears to fall short of this potential (Ferré-Bigorra et al., 2022; Patel et al., 2024; Stufano Melone et al., 2025). Our contribution provides a critical assessment of the application of urban DTs, comparing their theoretical potential for sustainable development with the limitations and tensions affecting sustainability outcomes that have been observed in their practical implementation.

Drawing on a review of recent literature and case studies highlighting successful and problematic implementations, we analyse digital transformation initiatives, with a focus on the co-creation of digital technologies. We identify discrepancies between aspirational goals, such as holistic systems thinking and citizen engagement, and realised functionalities, which are often focused on infrastructure management and operational efficiency. The aim is to raise awareness of unintended social and ecological effects in urban DT initiatives and foster discussions for a more reflective modelling process.

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  • Helbing, D. and Sánchez-Vaquerizo, J. A. (2023). ‘Digital twins: potentials, ethical issues and limitations’, In Handbook on the Politics and Governance of Big Data and Artificial Intelligence: Edward Elgar Publishing, 64–104.
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  • Stufano Melone, M. R., Borgo, S. and Camarda, D. (2025). ‘Digital Twins Facing the Complexity of the City: Some Critical Remarks’. Sustainability, 17, 3189.
  • Weil, C., Bibri, S. E., Longchamp, R., Golay, F. and Alahi, A. (2023). ‘Urban Digital Twin Challenges: A Systematic Review and Perspectives for Sustainable Smart Cities’. Sustainable Cities and Society, 99, 104862.

How to cite: Niehoff, S., Beier, G., Reißig, M., and Kunkel, S.: Is there a Gap Between Promise and Practice? A Critical Assessment of Digital Twins for Sustainable and Resilient Smart Cities , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17873, https://doi.org/10.5194/egusphere-egu26-17873, 2026.

EGU26-17959 | ECS | Posters on site | ERE6.2

The use of magnetotelluric and gravity studies to identify geothermal conditions – case study from the Polish Lowlands 

Anna Wachowicz-Pyzik, Adam Cygal, and Michał Stefaniuk

Geothermal potential in Poland is mostly associates with low-temperature resources accumulated in four geothermal provinces: Polish Lowlands, Carpathians, Carpathians Foredeep and Sudetes Region. Each provinces is characterized by different geological, and geothermal parameters, determination of which can be supported by magnetotelluric and gravimetric data. Magnetotelluric methods are frequently used as auxiliary under Polish conditions predominant by geothermal resources associated with sedimentary complexes and predominantly in resources connected with crystalline rocks, where seismic method is not effective. Gravimetric methods are used to identify deep and shallow fault zones, which may correspond to geothermal hotspots.

The paper presents examples of hydrogeothermal investigation supported by those two methods in Jurassic sedimentary complexes of Polish Lowlands. The results clearly shows that magnetotelluric and gravimetric methods can effectively support the selection of perspective areas for future low-temperature geothermal investments.

An integrated interpretation of magnetotelluric, gravimetric and seismic results (where available) in the exploration area, supported by existing hydrogeological data, improves the reliability of conceptual models of geothermal systems in the Polish Lowlands by reducing interpretational ambiguity. Comprehensive interpretation helps to distinguish conductive zones related to saline aquifers from structural features controlling fluid circulation, such as fault and fracture zones. This approach reduces exploration risk at the early stage of project development by narrowing the target area for detailed surveys and by constraining the location and expected depth of exploratory wells. In practice, the proposed workflow can be used as a cost-effective screening tool to identify the most promising sites for low-temperature geothermal heat production.

How to cite: Wachowicz-Pyzik, A., Cygal, A., and Stefaniuk, M.: The use of magnetotelluric and gravity studies to identify geothermal conditions – case study from the Polish Lowlands, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17959, https://doi.org/10.5194/egusphere-egu26-17959, 2026.

EGU26-18464 | Orals | ERE6.2

A Transdisciplinary Approach to Urban Air Quality Research 

Erika von Schneidemesser, Seán Schmitz, Alexandre Caseiro, Lisa Blyth, and Andreas Kerschbaumer

Urban areas are focal points of resource consumption, innovation, and governance, but they are also hotspots where environmental stressors such as air pollution and climate change impacts disproportionately affect human health and ecosystem resilience. Improving urban air quality is therefore a central challenge for transformations to sustainable and resilient cities. In Berlin, Germany, a series of mobility-related laws enacted over the past five years aim to transform the city’s transport system toward greater environmental sustainability and climate neutrality. However, due to Berlin’s size, historical development, and fragmented governance structures, these measures—such as new bicycle lanes and temporary street closures—are implemented incrementally across diverse urban districts, complicating the assessment of their localized environmental impacts.

Using the transdisciplinary research approach of the Research Institute for Sustainability (RIFS) at GFZ, measurement campaigns to accompany policy implementations were co-designed with local stakeholders from the Berlin Senate Department for the Environment, Urban Mobility, Consumer Protection and Climate Action (SenUMVK). This research contributed to broader evaluations of the policy implementations and the decision-making processes in the city. Building on these experiences, at a larger scale, a similar transdisciplinary approach was implemented as the foundation for Net4Cities, a project with the aim of facilitating the realization of the EU Green Deal’s Zero Pollution Action Plan by advancing air and noise pollution monitoring infrastructure and providing evidence-based support for implementing effective transport policies and thereby improving air quality and mitigating noise pollution. A harmonized transdisciplinary approach was developed and applied during the first year of the project to build on and establish relationships with the 11 partner cities. This approach formed the basis for the project, and in line with the localized Berlin work, was designed to facilitate exchange among the project and partner cities, integrate interests and perspectives from science and policy stakeholders, and increase uptake and the utility of the project outputs. The presentation will discuss the transdisciplinary framework, its application, how this influenced the results and their uptake, as well as reflections on such an approach to influence transformation processes. This contribution highlights how transdisciplinary research can support the monitoring and mitigation of urban environmental stressors, address synergies between air quality improvement and climate action, and facilitate the uptake of scientific evidence into urban policymaking processes.

How to cite: von Schneidemesser, E., Schmitz, S., Caseiro, A., Blyth, L., and Kerschbaumer, A.: A Transdisciplinary Approach to Urban Air Quality Research, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18464, https://doi.org/10.5194/egusphere-egu26-18464, 2026.

EGU26-18661 | ECS | Posters on site | ERE6.2

Tools for Compatibility Screening in Shallow Subsurface Uses via Integrated Geophysical Ground Modelling with Uncertainty Assessment 

Adam Cygal, Gabriel Ząbek, Michał Stefaniuk, and Tomasz Maćkowski

Geophysical surveys are widely used to characterize lithological and structural variability in the subsurface. They support the design of shallow, low-temperature geothermal systems, the delineation of freshwater aquifers, and the assessment of investment risk associated with subsurface interventions. Evidence from the authors’ projects and from published case studies shows that a detailed ground model is central to environmental impact assessment, definition of technical boundary conditions, and planning of synergies between operation and its interactions with existing infrastructure, local communities, and the natural environment. In practice, this requires translating interpretation results into project-relevant parameters, including lithology distribution, layer thickness, key boundary geometries, disturbed zones, and hydrogeological conditions, together with risk indicators that describe the likelihood of adverse ground and groundwater conditions at the planned site. Interpretation remains challenging because ambiguity arises from limited resolution and survey coverage and from the inherent heterogeneity of unconsolidated sediments.
This paper presents an integrated workflow for shallow investigations that combines seismic, electrical resistivity and electromagnetic methods to reduce ambiguity through consistent multi-method integration and explicit uncertainty quantification. The workflow assumes that the geological model must both respect method-specific limitations and represent the subsurface architecture realistically enough to support engineering decisions. Spatial geostatistical modelling is used to capture variability and to propagate uncertainty into maps and cross-sections of key boundaries and properties. Geostatistical and Artificial Intelligence tools support data fusion, recognition of structural features and lithological zones, and systematic comparison of alternative geological scenarios. The resulting ground model is delivered as a most-likely realization accompanied by uncertainty products, including probability-based representations of lithology and confidence intervals for boundary positions, so that the outputs can be used directly in technical and environmental risk assessment and in selecting the preferred design variant.
The workflow is demonstrated on experimental field data collected during a seismic project carried out in Poland, in an area with unfavorable geological conditions that generate highly ambiguous seismic responses. Although the survey was not originally intended for shallow geothermal design, it enabled development and testing of the integrated workflow and the formulation of practical guidance for siting shallow installations. The study focuses on ambiguity drivers such as strong attenuation and scattering in unconsolidated deposits, lateral and vertical velocity variability, and locally changing saturation, and on mitigation measures based on survey design, processing choices, and integration with electrical methods. The site is representative of settings with heterogeneous Quaternary cover and thick unconsolidated sediments under variable hydrogeological conditions, which also supports transfer of the methodology to the exploration and characterization of shallow freshwater resources. The final outcome is a coherent methodological description and decision oriented recommendations that support transparent, defensible assumptions during planning and implementation under uncertainty.

How to cite: Cygal, A., Ząbek, G., Stefaniuk, M., and Maćkowski, T.: Tools for Compatibility Screening in Shallow Subsurface Uses via Integrated Geophysical Ground Modelling with Uncertainty Assessment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18661, https://doi.org/10.5194/egusphere-egu26-18661, 2026.

EGU26-19355 | ECS | Orals | ERE6.2

Earth-to-Air Heat Exchangers and Their Role in Energy Efficiency of Large-Scale Buildings 

Marta Czapka and Michał Kaczmarczyk

In this paper, the role of Earth-to-Air Heat Exchangers (EAHEs) in improving the energy efficiency of large-scale buildings is examined. Particular attention is given to its applicability in facilities, where high ventilation rates, large internal volumes, long operating hours, and the frequent need for air quality control create favorable conditions for upstream air tempering. Integration pathways are outlined in relation to typical ventilation architectures and control strategies, emphasizing the potential for demand reduction under design conditions and improved part-load performance during seasonal operation.

Finally, EAHEs are positioned within broader sustainable energy management strategies for logistics buildings, including hybrid configurations with heat recovery ventilation, heat pumps, and renewable energy systems. The potential contribution of EAHEs to operational energy reduction and associated emissions mitigation is discussed, while noting that robust performance assessment requires careful consideration of site-specific constraints and the use of dynamic simulation and monitoring frameworks to support design optimization and verification.

How to cite: Czapka, M. and Kaczmarczyk, M.: Earth-to-Air Heat Exchangers and Their Role in Energy Efficiency of Large-Scale Buildings, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19355, https://doi.org/10.5194/egusphere-egu26-19355, 2026.

EGU26-19410 | Posters on site | ERE6.2

Analysis of the Possibility of Recognizing the Deep Geological Structure of the Krakow Region for Advanced Geothermal Systems (Ags) Implementation 

Michał Stefaniuk, Konrad Lukaj, Anna Wachowicz-Pyzik, Adam Cygal, Ryszard Hodiak, and Marcin Nowak

Geothermal energy in Poland is currently used primarily for heating purposes, with an increasing emphasis on recreational and therapeutic applications. These trends are particularly evident in the southern part of the country, in the Małopolska Voivodeship. Geothermal waters occurring in the porous-fissure aquifer of the Podhale Basin are characterized by high flow rates, temperatures close do 90oC  and low mineralization.
Advanced Geothermal Systems (AGS) may prove a significant opportunity for utilizing geothermal resources in the coming years. These systems utilize closed-loop heat systems, in which the medium circulates in a closed system, transferring energy stored in the deep, hot layers of the earth crust to the surface. The implementation of AGS requires reservoirs with temperatures exceeding 100 °C, high thermal conductivity, and very low natural permeability. This creates an opportunity for the deployment of such systems in areas with high energy demand, especially for district heating applications, where natural hydrogeothermal resources with suitable temperature and flow characteristics are absent. A potential recipient in the Małopolska Voivodeship is Kraków, second largest city in Poland with population around 800,000, whose area is geologically poorly explored due to its dense development and lack of hydrocarbon deposits. Consequently, no detailed seismic surveys have been conducted in this region. As a result, significant uncertainties exist regarding the thickness of the overlying sedimentary sequences, the depth of the crystalline basement, its petrophysical properties, and the structural configuration of fault zones. To determine the feasibility of implementing an AGS system, an attempt was made to analyze the possibilities of geological exploration for the Kraków region by designing geophysical surveys along seismic profiles, which would enable the identification of deep geological structures.

How to cite: Stefaniuk, M., Lukaj, K., Wachowicz-Pyzik, A., Cygal, A., Hodiak, R., and Nowak, M.: Analysis of the Possibility of Recognizing the Deep Geological Structure of the Krakow Region for Advanced Geothermal Systems (Ags) Implementation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19410, https://doi.org/10.5194/egusphere-egu26-19410, 2026.

EGU26-19673 | ECS | Orals | ERE6.2

Assessment of Geo-methanation Potential from Biogenic CO2 inAustria under Renewable Electricity Constraints 

Patrick Jasek, Gerald Stiedl, and Ott Holger

Austria’s energy system is characterised by a high share of bioenergy, resulting in substantial biogenic
CO2 emissions from industrial and energy-sector point sources. These emissions represent a potential
carbon feedstock for geo-methanation, enabling the production of renewable methane that is compatible with
existing gas infrastructure. This study presents a national-scale assessment of Austria’s geo-methanation
potential by integrating (i) a spatially resolved inventory of biogenic CO2 point sources, (ii) benchmarked
capture efficiencies by sector, (iii) green hydrogen production constrained by surplus renewable electricity
and electrolyser deployment, and (iv) experimentally observed biological methane yields. Results indicate
that 9–12 Mt CO2 a−1 of biogenic point-source emissions occur nationally, of which 5–8 Mt CO2 a−1 are
technically capturable [1, 2]. Using Austria’s net electricity export balance of 6.8 TWh a−1-derived from
annual import–export statistics, as an upper-bound proxy for surplus electricity, ∼0.7 Mt CO2 a−1 could
currently be methanated [3]. Laboratory geo-methanation experiments achieving approximately 20 % of the
stoichiometric methane yield reduce the methane output potential to 5–8 TWh a−1, corresponding to 7–11 %
of Austria’s current natural gas demand [4, 5]. A phased ramp-up strategy is proposed to reach 10 %, 25 %,
and 50 % utilisation of the biogenic CO2 pool through progressive electrolyser deployment and renewable
electricity expansion. The results demonstrate that Austria’s geo-methanation potential is fundamentally
constrained by the availability of renewable electricity and hydrogen, rather than CO2 supply.

How to cite: Jasek, P., Stiedl, G., and Holger, O.: Assessment of Geo-methanation Potential from Biogenic CO2 inAustria under Renewable Electricity Constraints, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19673, https://doi.org/10.5194/egusphere-egu26-19673, 2026.

EGU26-19906 | ECS | Orals | ERE6.2

Pore Structure Development and Mechanical Degradation of Sandstone Under Thermal Loading for Geotechnical Applications 

Arijit Sahoo, Amit Kumar Verma, Ashutosh Tripathy, and Trilok Nath Singh

Understanding the mechanical deformation and pore characteristics of sandstone at high temperatures is crucial for optimizing its application in subsurface energy systems such as Geological carbon sequestration, underground coal gasification (UCG), and geothermal energy extraction. In this research, the impact of mild heat exposure on the mechanical properties and pore structure of sandstone from the Barakar Formation, Jharia Basin, India, was investigated. Low-pressure gas adsorption (LPGA), helium pycnometry, and water immersion porosimetry (WIP) were used to measure porosity and pore evolution quantitatively. Brazilian tensile strength (BTS) and uniaxial compressive strength (UCS) tests were used to assess the mechanical performance of the sandstone with temperatures. 

Low-Pressure Gas Adsorption (LPGA) investigations reveal the presence of silt-shaped pores in the studied samples. Both the specific surface area and pore volume increase with an increase in temperature. Additionally, WIP and He pycnometer data indicate that porosity increases with an increase in temperature, although the change is not significant. BTS and UCS data show a steady decrease in strength characteristics with rising temperatures. This degradation is attributed to the creation of microcracks, the enlargement of pre-existing pores, and thermally driven mineral changes. The study emphasizes the importance of considering thermal effects in subterranean reservoir planning and geotechnical systems, particularly in assessing long-term stability and safety in thermally active environments.

How to cite: Sahoo, A., Verma, A. K., Tripathy, A., and Singh, T. N.: Pore Structure Development and Mechanical Degradation of Sandstone Under Thermal Loading for Geotechnical Applications, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19906, https://doi.org/10.5194/egusphere-egu26-19906, 2026.

EGU26-19923 | ECS | Orals | ERE6.2

Beyond Pilots: Urban Digital Platforms as Enduring Research Infrastructures 

Leila Javanmardi and Tim Fraske

Urban digital platforms (UDPs) increasingly mediate how cities are governed, which services are provided, and to what extent citizens engage in urban life. A growing body of research—often discussed under the label of platform urbanism—has explored the development of UDPs in urban studies, however mostly in relation to phenomena such as the gig economy, short-term rentals, and platform-mediated urban services as profit-driven corporate tools.

This article instead focuses on a smaller but increasingly important category of UDPs developed by municipalities, research institutions, and civic actors, aimed at functioning as  supporting elements for decision-making. Designed for planning, participation, and co-design, these platforms, however, often remain temporary pilots rather than evolving into infrastructures for sustained collaboration and reflexive governance. Therefore, our research question is as follows: how can UDPs be technically designed and institutionally embedded so that they evolve from pilots into infrastructures and support long-term, reflexive urban governance?

Here we conceptualize UDPs as research infrastructures for transformation-oriented urban research: socio-technical arrangements that organize how knowledge is generated, validated, and circulated in cities, laying the groundwork for more democratic, just, and sustainable urban co-production. Drawing on German experiences with Real-world Labs (RwLs) as practice-oriented research settings—which have become central inter- and transdisciplinary arenas for addressing sustainability and urban transformation challenges—we identify three recurring dimensions that shape whether UDPs evolve into infrastructures: (1) their capacity to function as a science–policy interface enabling knowledge transfer across academic, political, and civic domains; (2) the risk of quantitative bias over qualitative insights, drawing boundaries on inclusion in decision-making and creating a struggle to accommodate the qualitative and contextual forms of knowledge that are equally vital for reflexive urban transformation; and (3) their role in institutional learning, particularly how organizational routines and governance structures adapt to embed experimentation over time.
These dimensions suggest that the future of UDPs depends not primarily on technical design but on their institutional embedding. As infrastructures of reflexive urban governance, they can support urban resilience and sustainable urban transformation if they balance efficiency with inclusivity and connect short-term experimentation to long-term urban change. Otherwise, digital urban futures risk being shaped predominantly by technocratic or corporate agendas.

How to cite: Javanmardi, L. and Fraske, T.: Beyond Pilots: Urban Digital Platforms as Enduring Research Infrastructures, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19923, https://doi.org/10.5194/egusphere-egu26-19923, 2026.

The subsurface (geological space beneath  Earth’s surface) is increasingly treated as a multifunctional resource that must serve multiple purposes in the era of the low-carbon economy. The most important current and near-future energy-related uses may include:
•    conventional and enhanced geothermal systems (EGS) 
•    low- and medium-temperature aquifer thermal energy storage (ATES) 
•    borehole thermal energy storage (BTES) 
•    underground hydrogen storage (porous reservoirs or salt caverns)
•    etc.
Exergy analysis offers a rational way to compare different applications while answering the question: how much useful energy could theoretically be obtained from each cubic meter of subsurface space used in a given way?
Purely volumetric approaches („how many m³ do we have?") can be very misleading – exergy density is usually a much better indicator of real resource value. In this view, priority should be given to high-exergy applications in the most valuable parts of the subsurface.  In the case of energy storage technologies, exergy loss is proportional to the entropy change due to heat dissipation to the environment. This effect will be greater the higher the temperature of the stored heat. The article considers temperature ranges typical for heat storage technologies.

How to cite: Pajak, L., Halaj, E., and Wachowicz-Pyzik, A.: A preliminary comparison of subsurface energy applications from the exergy perspective as a tool for sustainable use of subsurface resources assessment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19988, https://doi.org/10.5194/egusphere-egu26-19988, 2026.

EGU26-20020 | ECS | Orals | ERE6.2

Connecting Urban Transformation Labs to understand, anticipate and leverage resilient and sustainable cities and their surrounding areas 

Franziska Baack, Felix Brennecke, Annika Weiser, and Daniel Lang

Functional urban areas have to adapt to ever evolving challenges from climate change to digitalization to become sustainable and resilient. These complex transformation processes also require an evolution of scientific approaches. Towards this end, we explore the question: How can we better understand, anticipate, and enable transformations towards resilient and sustainable cities through interconnected Urban Transformation Lab research? In this paper we outline a comprehensive conceptual framework to guide the establishment and operation of 3-5 interconnected Urban Transformation Labs that shall be established in a multi-year approach in several cities in Germany run by several Helmholtz Centers. The framework is built on three central pillars: observation, simulation, and experimentation. The overarching goal is to use insights from urban observatories (pillar 1) gathering various environmental and spatial data as a basis for both the digital tools, such as simulation and visualizations (pillar 2), as well as the experimentation together with stakeholders in the real world (pillar 3). Ultimately, the conceptual framework will enable transferability of the approach as well as cross-case comparison between multiple labs in different contexts tackling a variety of challenges and employing a number of solutions.

How to cite: Baack, F., Brennecke, F., Weiser, A., and Lang, D.: Connecting Urban Transformation Labs to understand, anticipate and leverage resilient and sustainable cities and their surrounding areas, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20020, https://doi.org/10.5194/egusphere-egu26-20020, 2026.

EGU26-20062 | ECS | Posters on site | ERE6.2

Creative Mapping for Climate Adaptation: Two Case Studies from Jakarta´s Coast 

Teresa Erbach

Urban resilience in the face of climate change and increasing hydrometeorological risks depends not only on technical solutions, but also on social practices, local knowledge, and governance structures that shape how adaptation is understood and enacted. Although the importance of social and cultural dimensions in climate adaptation is widely recognised, there are still few approaches that explicitly address them. One approach that has gained increasing attention in recent years is the use of playful methods, particularly games. These approaches typically aim to foster civic engagement, community resilience, and adaptation literacy. Their playful nature creates space for participants to articulate concerns, desires, and tensions while granting them agency—an experience that can be both empowering and motivating.

Drawing on two case studies from Kampung Akuarium, a flood-prone coastal neighbourhood in Jakarta, we examine memory mapping with children and speculative gameplay involving residents and local government officials. These methods are discussed as experimental interfaces between lived experiences of environmental stressors and formal planning processes. We analyse their methodological affordances and limitations, particularly with regard to their capacity to open spaces for collective reflection on spatial transformation and to elicit social and cultural values, including emotional attachments, that are often excluded from technocratic planning.

Creative mapping enabled residents to document their own spatial narratives and experiences with recently implemented flood protection structures. It also revealed that the disconnection of local residents from their familiar environments reflects a broader shift in the cultural landscape of kampungs, where access to the sea has increasingly been restricted through redevelopment, protective infrastructure, and displacement. Aiming to (re)claim cartography as a means of situated storytelling and collective agency, the workshops sought to create spaces for articulating and negotiating relationships with the environment and for imagining alternative futures of life along the waterfront—an endeavour that proved only partially successful. While challenging technocratic mapping practices, the workshops also demonstrated that playful forms of mapping alone cannot counter the realities of spatial planning. They can document experiences and provoke reflection, but re-establishing access to space requires broader structural change. Without explicit links between workshop outcomes and institutional responsiveness, such mapping approaches risk remaining symbolic rather than transformative.

We argue for a context-sensitive and strategic deployment of creative mapping methods as part of broader socio-technical adaptation efforts. When embedded in sustained research and planning processes, they can contribute to more resilient urban futures by linking local knowledge and lived experiences with governance in rapidly transforming urban environments.

How to cite: Erbach, T.: Creative Mapping for Climate Adaptation: Two Case Studies from Jakarta´s Coast, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20062, https://doi.org/10.5194/egusphere-egu26-20062, 2026.

EGU26-20347 | ECS | Orals | ERE6.2

Navigating geothermal development for Singapore 

Jonathan Poh, Alessandro Romagnoli, Jian Wei Mark Lim, Tobias Massier, Anurag Chidire, Wei Wu, and Thomas Hamacher

Singapore relies heavily on energy imports to sustain urban development and ensure energy security, given its absence of extractable natural resources. Currently, natural gas dominates the energy mix. Singapore is considering several clean energy pathways to decarbonise and diversify, including solar photovoltaics, clean energy imports from neighbouring countries, hydrogen-ammonia, and nuclear power. Solar is among the most cost-effective domestic options, yet its extensive land requirements pose challenges for a land-scarce nation. By contrast, geothermal energy warrants investigation as a potential local low-carbon energy source, subject to the confirmation of sufficient subsurface heat resources.

Two deep exploratory slimholes were recently drilled in northern Singapore, reaching depths of 1.12 km and 1.76 km. Their bottom-hole temperatures measured 70°C and 122°C, respectively. From these results, geothermal gradients based on conductive heat transfer evaluated at 40–44°C/km. If such gradients persist to depths of 4–5 km, rock temperatures could exceed 200°C, enabling both electricity generation and direct-use applications. Scenario-based techno-economic and environmental assessments indicate that, if the high geothermal gradients inferred from recent drilling persist to greater depths, geothermal energy could become cost-competitive with existing electricity and cooling supply options under favourable development conditions. Competitiveness is contingent on substantial reductions in well development costs and the successful deployment of advanced subsurface heat-extraction concepts.

Despite these encouraging findings, geothermal remains a nascent technology in Singapore. Research and development are still at an early stage, though the recent drilling campaign marks a revival of efforts first initiated in 2002. Global technological advances in heat extraction and drilling are on the cusp of being demonstrated in the field. Successful deployment could serve as a model for other countries away from tectonic and volcanic settings. However, several challenges must be addressed in Singapore before geothermal can be fully realized. Chief among these are limited data availability and a shortage of local expertise. Building a robust talent pool and expanding the dataset are critical steps to reduce uncertainty and accelerate development. By overcoming these barriers, Singapore can strengthen its position to adopt and assist future geothermal within and in other neighbouring countries, complementing its broader clean energy strategy and enhancing long-term sustainability.

How to cite: Poh, J., Romagnoli, A., Lim, J. W. M., Massier, T., Chidire, A., Wu, W., and Hamacher, T.: Navigating geothermal development for Singapore, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20347, https://doi.org/10.5194/egusphere-egu26-20347, 2026.

EGU26-20579 | ECS | Orals | ERE6.2

A Model for sCO2 Storage in Superhot Geothermal Systems 

Christoph Scherounigg and Holger Ott

Superhot geothermal systems, characterized by pressures exceeding 22 MPa and temperatures above 374°C and therefore water being found in its supercritical state, offer a unique opportunity to integrate renewable energy production with carbon capture and storage (CCS). In these systems, supercritical CO2 (sCO2) has a higher density than water, enabling the formation of a sinking CO2 plume that minimizes leakage risks while simultaneously utilizing in-situ geothermal fluids for energy supply. In this presentation, we demonstrate our recent study on the dynamics of CO2 injection and migration in both unfractured, homogeneous, and fractured geothermal reservoirs. Our simulation workflow includes a stochastic fracture network generator that can incorporate various parameters, such as fracture dimensions, strike and dip angles, and fracture network restrictions. Furthermore, the exchange of heat and mass between fracture networks and the surrounding matrix was realized using transfer coefficients rather than a combined grid. This poses numerical challenges that will be discussed during the presentation.

In addition, results from selected simulation runs will be presented, based on different reservoir permeabilities and specific fracture network characteristics, regarding CO2 plume behavior, breakthrough dynamics, and temperature distributions within the reservoir. Overall, high permeability is favorable, while fractured reservoirs exhibit complex migration patterns. Temperature analysis confirmed minimal cooling effects, ensuring long-term operation. In conclusion, our study highlights the conditions necessary for combining CCS and superhot geothermal energy utilization and provides a 3D model for future evaluations.

How to cite: Scherounigg, C. and Ott, H.: A Model for sCO2 Storage in Superhot Geothermal Systems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20579, https://doi.org/10.5194/egusphere-egu26-20579, 2026.

EGU26-23206 | Posters on site | ERE6.2

Integration of Life Cycle Assessment for the Management of the Organic Fraction of Municipal Solid Waste (OFMSW) under a Circular Economy Approach 

Ana Paola Becerra Quiroz, Daniel Gil Ramírez2, María-Elena Rodrigo-Clavero, and Javier Rodrigo-Ilarri

Global municipal solid waste (MSW) generation reached 1.2 billion tonnes in 2022 and is projected to increase to 3.8 billion tonnes by 2050, driven mainly by urbanization and changes in consumption patterns (UNEP & ISWA). In Colombia, MSW generation amounted to 31.31 million tonnes in 2022, of which the organic fraction of MSW (OFMSW) represents between 36% and 58% of the total, depending on the urban context (DANE, 2024). The predominant disposal in sanitary landfills, combined with inadequate technical management, has generated critical environmental impacts, including the emission of nearly 20% of global anthropogenic methane (CH₄) (UNEP, 2021), a gas with a global warming potential approximately 80 times higher than CO₂ (Calvin et al., 2023), as well as the production of highly contaminating leachates and risks to public health (UNEP, 2021).

A paradigm shift has recently been identified, moving from linear collection-and-disposal schemes toward circular-economy-based energy recovery models, in which advanced Mechanical–Biological Treatment (MBT) technologies (Nanda & Berruti, 2021)—including anaerobic digestion (AD), advanced composting, co-digestion, gasification, and pyrolysis—enable the transformation of OFMSW into biogas, bioenergy, and other bioproducts, thereby reducing pressure on final disposal systems and contributing to the achievement of the Sustainable Development Goals (SDGs) (Sharma et al., 2021; Nanda, 2021).

This research is grounded in the formulation of integrated OFMSW management models that consider the physicochemical characterization of waste, which serves as the basis for technology selection and performance assessment (Sondh et al., 2024). Within this framework, Life Cycle Assessment (LCA) is applied to quantify the environmental impacts associated with the implementation of these treatment technologies, and multi-criteria decision-making tools are incorporated to integrate technical, economic, and social variables, enabling comparative scenario evaluations among emerging technologies with the aim of maximizing OFMSW valorization under circular economy principles.

It is estimated that technified OFMSW management could contribute to a potential reduction of 29 to 57 million tonnes of CH₄ emissions globally by 2030 (UNEP, 2021). In Colombia, the implementation of MBT systems for at least 5% of OFMSW, combined with biogas utilization, constitutes a key strategy for the country to achieve its target of a 51% reduction in greenhouse gas emissions by 2030 (Minambiente, 2020). Likewise, the energy recovery of OFMSW provides a strategic contribution to the energy security of Latin American megacities during drought periods, reducing dependence on conventional thermoelectric sources (Sond et al., 2024). Consequently, integrated OFMSW management based on LCA has the potential to reduce environmental impacts and public health risks, transforming waste into assets for resilient urban development.

 

How to cite: Becerra Quiroz, A. P., Ramírez2, D. G., Rodrigo-Clavero, M.-E., and Rodrigo-Ilarri, J.: Integration of Life Cycle Assessment for the Management of the Organic Fraction of Municipal Solid Waste (OFMSW) under a Circular Economy Approach, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-23206, https://doi.org/10.5194/egusphere-egu26-23206, 2026.

The planning and management of multiple dams within a river basin are critically important for the effective use of water resources and energy generation. Under the growing pressures of climate change, Türkiye, classified as a water-stressed region, faces significant challenges in balancing water availability with population growth, environmental sustainability, and energy demands. The sustainable operation of multiple dams is a vital step toward ensuring the efficient utilisation of water resources for the country's future, while addressing environmental considerations and climate resilience.

The Euphrates-Tigris Basin spans a semi-arid area of 762,000 km², covering six countries: Türkiye, Iran, Iraq, Jordan, Syria, and Saudi Arabia. The two major rivers in the basin, the Tigris and Euphrates, originate from the mountains in eastern Türkiye. These rivers are primarily fed by snowmelt stored during the winter, while during the dry summer months, they rely heavily on groundwater, making the region particularly vulnerable to climate change. Approximately 60 million people depend on these rivers for irrigation, energy production, and other water-related needs. This study focuses on the portion of the Euphrates-Tigris Basin located within Türkiye, covering an area of 18,500 km² (Esit et al., 2023; Rateb et al., 2021).

Türkiye has built 19 hydropower plants and 22 dams in this region over recent decades to store water for irrigation, energy generation, and flood control (SAPRDA, 2009). However, the basin faces increasing challenges due to climate change, including reduced precipitation, rising temperatures, and greater variability in seasonal water availability. These changes exacerbate flood risks during extreme rainfall events while also intensifying drought conditions in dry seasons. The stored water in dams is essential for hydropower production, contributing to Türkiye’s renewable energy targets, yet evaporation losses and reduced inflows pose threats to long-term sustainability. Addressing these interconnected issues is critical for maintaining water security, energy production, and ecosystem stability in the region.

Currently, dams in Türkiye are operated individually, often without coordination or consideration for downstream interdependencies, population growth, or the effects of a changing climate. Using the Euphrates- Tigris basin as a case study, this study seeks to explore the impacts of multiple dam operations in water management. The research will analyse the implications of uncoordinated dam operations on water allocation, seasonal water availability, and hydropower production. Furthermore, it will assess the potential benefits of integrated dam management strategies for improving water resource efficiency. By identifying key challenges and opportunities, this study aims to contribute to the sustainable management of the Euphrates-Tigris Basin in the face of evolving climatic and socio-economic pressures.

How to cite: Sarışen, D. and Yılmaz, D.: Managing Water Resources in the Euphrates -Tigris Basin: Impacts of Multipurpose Dam Operations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4546, https://doi.org/10.5194/egusphere-egu26-4546, 2026.

EGU26-5116 | ECS | PICO | HS2.2.9

Impacts of the Kapulukaya Dam on the Hydrological Health of the Kızılırmak River 

Arda Enes Yıldırım and Döndü Sarışen

This study analyzes the hydrological conditions of the downstream of Kapulukaya Dam on the Kızılırmak River, comparing the pre-construction natural period (1970–1989) with the post-operation-controlled period (1989–2013). Using the Flow Health Software, the nine different hydrological sub-indicators, such as High Flow, Low Flow, and Seasonal Flow Shift were employed to determine the ecological and functional integrity of the river on a scale of 0 to 1. The results show a moderate deviation from natural processes; the most significant changes were observed in the Flood Flow Interval (FFI) and Seasonal Flow Shift (SFS) indices, indicating the suppression of natural flood cycles. Even during periods of extreme drought between 2006 and 2008, the Kapulukaya Dam has a high Persistently Very Low (PVL) rating of 0.95, preventing the complete drying up of the riverbed. However, the facility failed to reach its design energy production target of 190 GWh annually due to climatic pressures and upstream water conditioning. Furthermore, factors such as increase in drinking water demand in Kırıkkale and the lack of a central irrigation union negatively affected operational efficiency. The results obtained demonstrate that the dam achieved its flood control objective but experienced increased seasonal pressures on the river flow. In conclusion, the study highlights the need for an efficient water management strategy in the Kızılırmak Basin, encompassing climate change and water demand scenarios to achieve long-term sustainability.

How to cite: Yıldırım, A. E. and Sarışen, D.: Impacts of the Kapulukaya Dam on the Hydrological Health of the Kızılırmak River, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5116, https://doi.org/10.5194/egusphere-egu26-5116, 2026.

EGU26-5184 | PICO | HS2.2.9

A web-based integrated Hydrosphere modeling system for scientists and decision-makers 

Lluís Pesquer, Amanda Batlle, Savitri Galiana, Xavier Garcia, Kaori Otsu, Eva Flo, Ester Prat, Elisa Berdalet, and Joaquim Ballabrera

The appropriate management of the water system requires a holistic consideration of the inland waters, the marine ecosystems and their interactions. However, these two systems are monitored, analysed and modelled separately and managed with often non connected policies. This is in part due to the intrinsic characteristics of the two systems and to the complex processes occurring between them, usually understudied. Nowadays modelling offers new opportunities for integrating land-sea interactions, as we show in this study. At the same time, such models are expanding their capabilities in cloud computing environments. However, many existing modelling tools remain fragmented and are limited to either inland or marine components, such as Digital Twin Earth (DTE) Hydrology Next or European Digital Twin Ocean (EDITO). To overcome this limitation, the current work presents a virtual research environment (VRE)-based workflow with a single interface for the whole water continuum: from inland water, through coastal water to open oceans. We present a seamlessly connected inland surface hydrological model with a modular ocean circulation modelling system, available into the AquaINFRA VRE in compliance with FAIR principles. It is provided on the web-based Galaxy platform https://aqua.usegalaxy.eu/ to facilitate the integration with the European Open Science Cloud (EOSC) system.

The developed solution allows to execute the modelling workflow in a pre-prepared specific region with a chain of three components:

  • Surface inland model: it allows different scenario simulations at daily or monthly responses through parameterised SWAT+ executions with a previous watershed delineation.
  • Inland-marine connector: transform the output in hydrological response units in the neighbouring of the mouth in the sea of the catchment area to needed inputs for the marine model.
  • Ocean circulation model: it takes as input for the rivers and computes with the MITgcm modelling code the coastal ocean dynamics.

This workflow is initially developed for a Mediterranean use case but is designed to be reproducible and scalable to other European and global regions. The first study area tested is the Tordera catchment and its neighbouring coastal zone, located on the central Catalan coast in the NW Mediterranean. The Tordera basin features a diverse landscape, including croplands, shrublands, forests, urban areas, and industrial zones. Associated human activities, together with the high variability of climatic events, directly affect the quantity and quality of water in both inland and marine ecosystems. Therefore, integrated information through the water continuum is key for its management.

The proposed system aims to 1) reduce the technical complexity of hydrological and marine model executions, 2) show an innovative connection tool between fresh and ocean water environments, and 3) display clear and useful information of the results. The AquaINFRA project will make this system accessible to a broader research community beyond SWAT and MITgcm experts. Thus, scientists, decision-makers and other stakeholders will be able to simulate and assess different future scenarios and better understand past extreme events with an improved representation of land–sea interactions.

Acknowledgments

The AquaINFRA project received funding from the European Commission’s Horizon Europe Research and Innovation programme under grant agreement No 101094434

How to cite: Pesquer, L., Batlle, A., Galiana, S., Garcia, X., Otsu, K., Flo, E., Prat, E., Berdalet, E., and Ballabrera, J.: A web-based integrated Hydrosphere modeling system for scientists and decision-makers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5184, https://doi.org/10.5194/egusphere-egu26-5184, 2026.

With the increasing impacts of climate change in recent decades, numerous studies have reported a rising frequency of extreme rainfall events worldwide, accompanied by intensified droughts and floods. Consequently, traditional hydrological analyses require further consideration of climate change effects.This study analyzes more than 125-year record of daily rainfall observations (1900–2025) from the Taipei and Tainan meteorological stations in Taiwan. The dataset is divided into a historical period (1900–1990) and a recent period (1991–2025) to investigate long-term variations in extreme rainfall and drought characteristics. Three hydrological indicators are examined: (1) changes in return periods of extreme rainfall, (2) trends in the number of non-rainy days, and (3) months of extreme precipitation occurrence.In the return period analysis, the Annual Maximum Series (AMS) method combined with the Weibull plotting position formula was applied. The results reveal a decreasing trend in return periods at both the Taipei and Tainan stations, indicating an increased frequency of extreme rainfall events.In terms of drought characteristics, long-term variations in non-rainy days were examined based on the concept of an accelerated hydrological cycles. The results show that the number of non-rainy days has increased at a rate of approximately 0.3 days per year in both northern and southern Taiwan. Furthermore, the average annual number of non-rainy days in the recent period increased by approximately 23 days compared to the historical period, reflecting climate characteristics associated with reduced light rainfall and intensified drought–flood extremes.Regarding seasonal variability, the probability distribution of extreme precipitation occurrence by month was analyzed. The Taipei station exhibits an expansion of the flood season, with extreme precipitation events primarily occurring in June and October, forming a bimodal distribution. In contrast, the Tainan station shows a pronounced concentration of extreme precipitation during the wet season, with approximately 43.8% of events occurring in August.Based on these findings, it is recommended that flood control design standards be upgraded to account for shortened return periods of extreme rainfall. In addition, water resource allocation and management strategies should be strengthened to mitigate the increasing risk of water shortages associated with the rise in non-rainy days. Flood warning systems and construction planning should also be dynamically adjusted in response to shifts in the occurrence months of extreme precipitation.

How to cite: Yang, C.-L. and Lin, Y.-C.: Investigating Trends in Regional Hydrological Characteristics Under Climate Change Using Long-term Rainfall Observation Data: A Case Study of Taipei and Tainan, Taiwan, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6106, https://doi.org/10.5194/egusphere-egu26-6106, 2026.

Abstract: Under the increasing pressure of water scarcity, irrigation decision-making plays a critical role in achieving efficient agricultural water use while maintaining stable and increased crop yields. With the continuous advancement of crop water information sensing technologies, irrigation decisions based on multi-source farmland information monitoring have become an important development direction for precision irrigation. Targeting salinized farmland in arid regions with shallow groundwater tables, this study proposes an irrigation decision-making method based on in situ measured farmland evapotranspiration, which effectively avoids the adverse effects of soil salinity on the measurement accuracy of soil moisture sensors and enables precise irrigation regulation under saline conditions. Based on two consecutive years of comparative irrigation decision experiments conducted on tomato and maize, the results indicate that, compared with conventional soil-moisture-based irrigation decision methods, the proposed approach can reduce irrigation water use by 7.69%–14.29% while increasing crop yield by 19.6%–24.2%, leading to a significant improvement in crop water productivity. Furthermore, under the same decision-making framework, the use of plastic mulching combined with a moderate reduction in irrigation level (irrigation adjustment coefficient reduced from 0.9 to 0.7) further saved approximately 3.6%–9.8% of irrigation water and enhanced water productivity by 4.6%–33.5%. These results confirm the feasibility and advantages of the proposed irrigation decision method for salinized farmland and provide reliable theoretical support and empirical evidence for irrigation management and the development of smart irrigation technologies in arid salinized agricultural regions, with practical significance for advancing precision agriculture.

Keywords: irrigation decision-making; evapotranspiration

How to cite: Bingbing, J. and Zailin, H.: Research on Irrigation Decision-making Method for Salinized Farmland Based on Actual Farmland Water Consumption Monitoring , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9361, https://doi.org/10.5194/egusphere-egu26-9361, 2026.

EGU26-15137 | PICO | HS2.2.9

Application of DWAT for inflow estimation in a data-scarce agricultural reservoir 

Seonmi Lee, Cheolhee Jang, Deokhwan Kim, Wonjin Jang, Min-Gi Jeon, and Hyeonjun Kim

Climate change has intensified drought conditions, and various approaches have been developed to ensure stable water supply using reservoirs. In South Korea, many agricultural reservoirs are monitored only in terms of storage (water level), while inflow data are not available. This limitation poses a challenge for developing drought response strategies, highlighting the need for methods to estimate reservoir inflow under data-scarce conditions.

In this study, we propose a methodology for estimating inflow scenarios for agricultural reservoirs using a physically based hydrological model constrained by observed storage (water level) data. As a case study, the Donghwa Reservoir, an agricultural reservoir located in the Seomjin River basin, was selected, and the Dynamic Water Resources Assessment Tool (DWAT) was applied. DWAT is a physically based hydrological model that represents surface water and groundwater processes and is widely used for water resources planning and management.

In the model setup, a prescribed time series of agricultural water withdrawals from May to September was applied, and catchment parameters were adjusted using observed reservoir storage data. The comparison between observed and simulated storage indicates that the model reasonably reproduces the overall variability and statistical characteristics of reservoir storage. However, there are limitations in directly representing artificial operational elements considered in actual reservoir management, such as flood control storage and water intake restrictions. Consequently, larger deviations between observed and simulated storage occurred during periods of extreme drought and flood between 2017 and 2020.

The proposed approach demonstrates the feasibility of estimating inflow scenarios for reservoirs without inflow measurements using a physically based hydrological model and provides a methodological basis for future drought analysis and the development of operational strategies for agricultural reservoirs.

Keyword: DWAT(Dynamic Water resources Assessment Tool), drought, agricultural reservoir, inflow estimation, storage-based calibration

Acknowledgement: This work was supported by Korea Environment Industry & Technology Institute(KEITI) through Aquatic Ecosystem Conservation Research Program, funded by Korea Ministry of Climate, Energy and Environment(MCEE) (RS-2025-02304832).

 

How to cite: Lee, S., Jang, C., Kim, D., Jang, W., Jeon, M.-G., and Kim, H.: Application of DWAT for inflow estimation in a data-scarce agricultural reservoir, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15137, https://doi.org/10.5194/egusphere-egu26-15137, 2026.

EGU26-15611 | ECS | PICO | HS2.2.9

Quantifying Drought Impacts on Reservoir Operations with DWAT: The Obong Reservoir Water Crisis 

Wonjin Jang, Hyeonjun Kim, Cheolhee Jang, Seonmi Lee, Min-Gi Jeon, and Deokhwan Kim

In September 2025, Obong Reservoir(supplying ~87% of the city’s domestic water) in Gangneung-si, South Korea experienced a severe drawdown that triggered citywide rationing. Reported effective storage fell to about 11% on 12 Sep 2025, with the water level near 99.5 m, only 7 m above the implied dead-water line. This case study applies the Dynamic Water Resources Assessment Tool (DWAT) to (i) reproduce the observed 09/2025 drawdown, (ii) diagnose dominant drivers of the low-water crisis, and (iii) quantify the rainfall threshold required for short-term recovery. DWAT is a hydrological modeling framework designed for water-resources assessment across diverse regions worldwide. It allowing detailed characterization of both short- and long-term hydrologic behavior. DWAT represents key processes such as surface runoff, groundwater flow, and human water use (e.g., irrigation and municipal withdrawals), supporting integrated evaluation of water availability and its movement through a watershed.

For reservoir operation, simulations incorporated spillway/outlet/intake characteristics, the stage–area–storage relationship, and time-varying withdrawal data reflecting operational conditions. The simulation period spanned from January 2023 to September 2025, including a one-year warm-up period and the major drought period affecting Gangneung. Results confirm that DWAT accurately reproduces the progressive water-level decline over multiple seasons, the sharp drawdown in late summer 2025, and the transition into the near dead-storage zone in both timing and magnitude. Water-balance diagnostics indicate that the Obong watershed is strongly storage-dependent (surface runoff is less than 3.4%), such that prolonged drought markedly reduces event-driven inflow, depletion of soil moisture and groundwater weakens baseflow support, and continued pumping accelerates reservoir water-level decline. Recovery experiments using the calibrated model show that reservoir stage can return to the normal operating range and that restoration of soil moisture and groundwater storage requires at least ~200 mm of rainfall.

Overall, the DWAT-based drought simulation demonstrates that DWAT is well suited for integrated drought assessment and reservoir operation analysis, providing a practical tool for diagnosing low-water crises and for identifying actionable recovery thresholds that can support emergency response planning and adaptive water-supply management under increasing hydroclimatic variability.

This work was supported by Korea Environment Industry & Technology Institute(KEITI) through Water Management Program for Drought Project, funded by Korea Ministry of Climate, Energy and Environment(MCEE).(2022003610002)

 

How to cite: Jang, W., Kim, H., Jang, C., Lee, S., Jeon, M.-G., and Kim, D.: Quantifying Drought Impacts on Reservoir Operations with DWAT: The Obong Reservoir Water Crisis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15611, https://doi.org/10.5194/egusphere-egu26-15611, 2026.

EGU26-15934 | ECS | PICO | HS2.2.9

Diagnosing contrasting runoff responses under similar soil moisture conditions using the DWAT model 

Min-Gi Jeon, Hyeonjun Kim, Choelhee Jang, Deokhwan Kim, Wonjin Jang, and Seonmi Lee

Soil moisture is widely used to describe catchment wetness conditions and to support drought-related hydrological interpretation. However, runoff responses under apparently similar soil moisture conditions can differ substantially across catchments and events, suggesting that soil moisture alone may not fully capture the processes controlling runoff generation. This study aims to diagnose the hydrological mechanisms associated with contrasting runoff responses under comparable soil moisture states using the process-based DWAT model. The analysis will use daily catchment-scale DWAT outputs including soil moisture, precipitation, total runoff, baseflow (groundwater flow), recharge, infiltration, and actual evapotranspiration for multiple catchments with contrasting hydrological characteristics. To enable consistent comparison across time, daily soil moisture will be transformed into percentile-based indicators to classify relative soil moisture states without directly implying absolute drought impacts. Runoff response will be quantified using event-based runoff ratios derived from simulated precipitation and discharge, and associated process indicators will be evaluated to interpret differences in runoff behavior. By separating soil moisture state from runoff response and leveraging internal model process variables, this work provides a structured framework to investigate why hydrological responses may diverge under similar dry conditions. The proposed approach is expected to support process understanding relevant for drought analysis and catchment-scale hydrological modeling.

This work was supported by Korea Environment Industry & Technology Institute(KEITI) through Aquatic Ecosystem Conservation Research Program, funded by Korea Ministry of Climate, Energy and Environment(MCEE). (RS-2025-02304832)

 

How to cite: Jeon, M.-G., Kim, H., Jang, C., Kim, D., Jang, W., and Lee, S.: Diagnosing contrasting runoff responses under similar soil moisture conditions using the DWAT model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15934, https://doi.org/10.5194/egusphere-egu26-15934, 2026.

EGU26-15973 | PICO | HS2.2.9

Component-wise Decomposition of Return Flow in Paddy Fields Based on DWAT Simulations 

Deokhwan Kim, Wonjin Jang, Min-Gi Jeon, Seonmi Lee, Cheolhee Jang, and Hyeonjun Kim

In paddy fields, both rainfall and irrigation water from reservoirs contribute interactively to the hydrological cycle. Quantitative decomposition of return flow based on its source is essential for efficient management of agricultural water. In this study, we employed the Dynamic Water Resources Assessment Tool (DWAT), a physically based semi-distributed model, to simulate major hydrological components in paddy fields including surface runoff, interflow, baseflow, infiltration, evapotranspiration, and water storage and separated them into rainfall and irrigation origin contributions.

The proposed component-wise decomposition framework enables spatio-temporal analysis of each hydrological process and uniquely allows monthly tracking of water storage by origin across soil and groundwater layers, providing a novel approach not explored in previous studies.

This framework can offer diagnostic insight into irrigation efficiency. For example, rapid conversion of irrigation water to surface runoff may indicate hydrological inefficiency, while effective utilization of rainfall implies potential for optimized supply operations. Such source-based decomposition provides a qualitative understanding of irrigation performance that cannot be inferred from return flow ratios alone.

This study can contribute to optimizing the operation of agricultural reservoirs and improving irrigation allocation policies, ultimately enhancing the sustainability of agricultural water use and supporting adaptive water resource management under increasing uncertainties driven by climate change.

This work was supported by Korea Environment Industry & Technology Institute(KEITI) through Aquatic Ecosystem Conservation Research Program, funded by Korea Ministry of Climate, Energy and Environment(MCEE). (RS-2025-02304832)

How to cite: Kim, D., Jang, W., Jeon, M.-G., Lee, S., Jang, C., and Kim, H.: Component-wise Decomposition of Return Flow in Paddy Fields Based on DWAT Simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15973, https://doi.org/10.5194/egusphere-egu26-15973, 2026.

Algal blooms are characterized by the mass proliferation of cyanobacteria in eutrophic water bodies under environmental conditions such as elevated water temperature and nutrient concentrations, thereby destabilizing aquatic ecosystems and degrading water quality. To quantitatively assess algal bloom occurrence, chlorophyll-a concentration is widely used as a representative water quality indicator reflecting eutrophication levels and algal biomass. In South Korea, algal blooms frequently occur during summer as elevated water temperatures and sustained nutrient inputs create conditions favorable for algal growth. In particular, the Four Major River basins of South Korea serve as primary drinking water sources and play a critical role in water resource management, making variations in chlorophyll-a concentrations an important indicator for the early identification of potential water quality deterioration. However, existing water quality monitoring systems rely primarily on in situ observations, which limits their ability to capture spatiotemporal variability across extensive river reaches.

As a foundational step to address these limitations, we developed and evaluated a machine learning–based model to estimate chlorophyll-a concentrations using Sentinel-2 satellite data in combination with in situ water quality observations. Satellite spectral information and water quality variables, including water temperature, dissolved oxygen (DO), and turbidity, were used as input features, and a Random Forest (RF) algorithm was applied to develop a chlorophyll-a concentration estimation model. Based on test set validation, the RF-based model achieved an R² of 0.737, an RMSE of 13.07 (mg/m³), and an MAE of 5.83 (mg/m³), showing a reasonable level of agreement with observed chlorophyll-a concentrations.

This study confirms the applicability of combining satellite remote sensing data with in situ water quality observations for estimating chlorophyll-a concentrations. In addition, we present an analysis framework that can be extended to short-term chlorophyll-a prediction by incorporating information from previous time steps. This approach can be used to estimate and predict changes in chlorophyll-a concentrations, providing information to support future water quality management and monitoring strategy development.

How to cite: Lee, S. and Lee, Y.: Estimating Chlorophyll-a Concentrations in South Korean Rivers: A Machine Learning Approach Using Satellite Imagery, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16175, https://doi.org/10.5194/egusphere-egu26-16175, 2026.

According to the standard CSN 75 1400 "Hydrological data of surface waters", M-day discharges are among the basic hydrological data. The Czech Hydrometeorological Institute is responsible for deriving and providing these basic hydrological data.

The objective of the research was to derive basic hydrological data of low flows for description of the hydrological regime, to propose new methodological procedures for deriving basic hydrological data, which include the long-term average discharge Qa and M-day discharges. These data are, among other things, the basis for decision-making of water authorities. Updated information of the hydrological regime will serve to improve planning in the water sector and will contribute to maintain and improve water management as a key commodity for preserving and increasing the quality of life.

The paper presents methodical approaches used to derive basic hydrological data of low flows in the network of water gauging stations in the Czech Republic. Statistical processing used a five-parameter log-normal distribution (LN5), which is essential for accurate representation of extreme values ​​in hydrology. Furthermore, the paper shows the input data that went into the derivation and presents the resulting database of basic hydrological data for unobserved catchments.

How to cite: Kukla, P. and Kourková, H.: Derivation of basic hydrological data (M-day discharges) for the reference period 1991–2020 in the Czech Republic, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16389, https://doi.org/10.5194/egusphere-egu26-16389, 2026.

Lake water quality monitoring in India faces a critical paradox—one where sub-daily or daily data needs are only met with sparse, annually available information. The largest publicly available water quality dataset in India is hosted by the Central Pollution Control Board (CPCB), which only provides annual maxima and minima for a few monitored quality parameters, providing no details on their intra-annual variability. To bridge this critical data gap, this analysis attempts to build a Satellite-based Monitoring approach, demonstrated for two India lakes- Lake Nainital, a source water body in Uttarakhand (0.438 km2 area) and Lake Sukhna, a wastewater receiving water body in Chandigarh (1.38 km2 area). Using Sentinel-2 imagery from 2016-2023, we reconstructed water quality values for 11 parameters of interest, including optically active (chlorophyll-a, turbidity, TSS, etc.) and optically inactive (electrical conductivity, fecal bacteria, BOD, etc.), derived on 3 separate grid sizes: 10m*10m, 20m*20m and 30m*30m. For Lake Nainital, lake quality was analysed for a 100m buffer zone around the water intake point and the following analyses were performed

(i) Seasonal Random Forest models were trained with CPCB ground-truth data, achieving promising predictive accuracy. In that, for Lake Nainital, winter served as the optimal period for nutritional monitoring with R2 values exceeding 0.9, whereas temperature prediction was most accurate in the monsoon (R2=0.93).  Fecal coliform demonstrated remarkable accuracy in summer (R2=0.90), in stark contrast to its diminished performance during the monsoon (R2=0.80). Sukhna exhibited contrasting seasonal dependencies: temperatures peaked in summer (R2=0.81), while electrical conductivity spiked in winter (R2=0.90). Also, BOD prediction enhanced significantly from summer (R2=0.66) to winter (R2=0.91).

(ii) Using Modified Robust Principal Component Analysis (MRPCA) Lake Naintial successfully diagnosed a single-factor dominance to multi-stressor complexity, e.g., during the COVID-19 pandemic in 2020 anthropogenic pressures temporarily eased then resurged with altered patterns. Further, the chronic nutrient impairment of Lake Sukhna was also diagnosed using this approach.

 

The advantages of the proposed satellite-based lake monitoring approach are significant- allowing water treatment plant operators to seasonally forecast coagulant demand fluctuations. This novel satellite-to-tap approach demonstrates an alternative future for water quality monitoring-one which need not rely on extensive grab sampling or sensor-based data as inputs. It also allows regulatory monitoring of chronically impaired lakes of the country and monitoring the upkeep of restored and rejuvenated lakes.

How to cite: Suchetana, B. and Nag, S.: Development of a Satellite-based Monitoring Approach for Augmenting Open-source Indian Lake Water Quality Datasets with Seasonal Information, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17803, https://doi.org/10.5194/egusphere-egu26-17803, 2026.

EGU26-20395 | ECS | PICO | HS2.2.9

Update of a regional groundwater model using an ensemble-based approach 

Cécile Coulon, Pierre Le Cointe, Nadia Amraoui, and Pascal Audigane

A groundwater model of the Tarn-et-Garonne department in southern France was updated and recalibrated using an ensemble-based approach to support short- to medium-term groundwater level forecasting. The model uses the MARTHE finite-difference groundwater modeling software (developed by the BRGM) to simulate groundwater flow, stream-aquifer interactions and groundwater and surface water withdrawals in a Quaternary alluvial aquifer system.  The model was originally developed to support local groundwater management and define allowable groundwater abstraction volumes. It was later coupled with the SURFEX land surface model (developed by the CNRM) and integrated into Aqui-FR, a French hydrometeorological modeling platform that provides groundwater level forecasts at a national scale. The model was last calibrated using data through 2015 and a trial-and-error approach. The update incorporated ten additional years of groundwater level, stream flow and pumping data, along with the latest recharge and surface runoff estimates generated by the SURFEX model. History matching then was performed using an iterative ensemble smoother to generate an ensemble of posterior parameter realizations that honor both expert knowledge and observed groundwater levels and stream flows. Using the posterior parameter ensemble, the uncertainty in various predictions of interest, including groundwater levels and standardized piezometric level indices, was evaluated at multiple locations across the study area. All analyses were implemented using a fully scripted workflow to facilitate future model updates and deployment of the workflow in other areas.

How to cite: Coulon, C., Le Cointe, P., Amraoui, N., and Audigane, P.: Update of a regional groundwater model using an ensemble-based approach, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20395, https://doi.org/10.5194/egusphere-egu26-20395, 2026.

EGU26-160 | ECS | Posters on site | ITS3.12/NP8.8

Hybrid Deep Learning Framework for Urban Land-Use Prediction and Scenario Modelling of Bangalore 

Dipansh Sah, Anita Gautam, and Bharath Haridas Aithal

India’s rapid urbanization in major metropolitan cities has triggered significant shifts in land-use patterns, exerting far-reaching effects on regional environmental balance and the future resilience of local ecosystems. Bangalore, as a major metropolitan, has expanded its paved surface, placing its ecological systems under significant stress. Standard methods for modelling land use often struggle with complex spatial and temporal connections. These approaches also tend to lack strength when it comes to creating forecasts based on data for extended scenarios. This research presents an innovative hybrid transformer-based framework designed to predict fine-scale urban land-use dynamics within the city of Bengaluru. The multi-temporal Land use data of Bangalore were derived from satellite image classification, alongside static and dynamic geospatial predictor variables, which were considered necessary for land use forecasting based on the literature review. The proposed model architecture is a hybrid that integrates the Convolutional Neural Networks (CNNs) for spatial feature extraction with a Transformer-based encoder, leveraging self-attention mechanisms to effectively capture complex spatio-temporal dependencies from the data.  A baseline model, using CNN encoders, has been successfully implemented and trained on the 2012-2023 dataset. Preliminary results yield a high overall accuracy and a Kappa score. The framework is designed to achieve state-of-the-art prediction accuracy by uniquely capturing both spatial and temporal dependencies. The evaluation focuses on key spatial metrics, where we project superior 'quantity' and 'allocation' agreement and a more accurate capture of the heterogeneous patterns of both 'infill' and 'expansion' growth. The validated framework will be used to simulate two critical future scenarios for Bangalore's development: a 'Business as Usual' (BAU) scenario based on historical trends and a policy-driven 'Sustainable Development' (SD) scenario. By providing geospatial forecasts of these radiating paths, this research will offer a dynamic decision-support tool, empowering planners to visualize and assess the long-term environmental and ecological impacts of future growth and to guide policy towards a more sustainable urban future.

Keywords: Deep Learning, Transformer, Convolutional Neural Networks, Classification

 
 

How to cite: Sah, D., Gautam, A., and Haridas Aithal, B.: Hybrid Deep Learning Framework for Urban Land-Use Prediction and Scenario Modelling of Bangalore, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-160, https://doi.org/10.5194/egusphere-egu26-160, 2026.

Understanding how configurations of urban land-use features influence the spatial concentration of property crimes is vital for developing evidence-based safety and planning strategies. This study evaluates the geospatial associations between eighteen distinct land-use features and three types of property crimes: robbery, burglary, and theft in Nashik, India. Using property crime records from 2022 and locations of land-use features extracted through the Google Maps API, the research integrates Kernel Density Estimation (KDE), Location Quotient (LQ), and Multiple Linear Regression (MLR) modelling to uncover spatial patterns and statistically significant relationships.

Using KDE, property crime subzones were identified to capture local-scale variations of property crimes and land-use features. LQ analyses revealed uneven geographic concentrations of property crimes and land-use features across subzones. MLR models revealed that several land-use features, including ATMs, banks, hospitals, police stations, recreational places, shops, and transit places, significantly influence property crime occurrences. However, the magnitude of influence varies across different types of property crimes. One-way ANOVA test results confirmed that the MLR models were statistically significant, validating the geospatial associations between property crimes and land-use features.

The findings underscore the importance of integrating spatial analytics with urban planning to enhance safety. By demonstrating how geospatial patterns of land-use features influence property crimes, this study contributes to urban geoscience research and provides actionable insights for urban planners, urban designers, and policymakers. Future research could extend the analysis to spatiotemporal patterns or apply the methodology to cities with different built environment morphologies.

How to cite: Kumbhre, A. and Bharule, S.: Geospatial Associations between Property Crimes and Land-use Features: A Case of Nashik, India, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-706, https://doi.org/10.5194/egusphere-egu26-706, 2026.

EGU26-1136 | ECS | Orals | ITS3.12/NP8.8

Modelling Urban Energy and Water Fluxes with SUEWS under Data-Scarce Conditions in Delhi, India 

Divya Thakur, Richard Dawson, and Chandrika Thulaseedharan Dhanya

Understanding local-scale surface energy and water fluxes is essential for assessing the impact of urbanization on local climate. The Surface Energy and Water Balance Scheme (SUEWS) is a widely used urban land surface model for simulating these fluxes at the neighbourhood scale. However, its application in rapidly urbanizing data-scarce regions such as Indian cities is challenging due to limited flux observations and urban surface data. With the aim to assess the performance of SUEWS in capturing the surface energy and water balance dynamics, we use satellite-derived inputs with the nearest neighbour image processing technique to represent land use land cover, urban morphology and surface characteristics. The study area comprises two locations in Delhi, each delineated into nine grids centered on an existing meteorological observation station. The model has been run for a decade, and its performance is evaluated with remote sensing proxies for surface energy fluxes and observations of temperature and relative humidity. Results show that SUEWS can reasonably capture the seasonal variation and magnitude of urban energy components despite using derived data products. The study highlights practical strategies for urban flux modelling in data-scarce regions and is crucial for providing insights that support evidence-based urban planning to mitigate the urban heat island effect and sustainable water management policies.

How to cite: Thakur, D., Dawson, R., and Dhanya, C. T.: Modelling Urban Energy and Water Fluxes with SUEWS under Data-Scarce Conditions in Delhi, India, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1136, https://doi.org/10.5194/egusphere-egu26-1136, 2026.

EGU26-1768 | ECS | Orals | ITS3.12/NP8.8

Urban Ventilation in Light-Wind Conditions 

Shuojun Mei, Shiyi Hu, and Ting Sun

Urban ventilation under light-wind conditions is a critical factor of thermal comfort and air quality in high-density cities, particularly during extreme heat events when synoptic forcing is weak. This study presents an integrated framework that combines city-scale wind mapping, large-eddy simulation (LES), neighborhood-scale pollutant dispersion analysis, and model parameterization to advance understanding and representation of urban ventilation processes in weak-wind regimes.

First, a city-scale wind mapping tool is developed for Guangzhou based on urban morphological parameters. The results reveal extensive low-wind-speed zones at pedestrian level, especially in high-density districts, indicating suppressed wind-driven ventilation and an increased reliance on buoyancy-induced airflow.

Second, high-resolution three-dimensional LES is conducted to investigate buoyancy-driven thermal plume dynamics under weak ambient winds. Validation against laboratory experiments demonstrates that the model accurately captures plume bending, vertical transport, and plume merging. The simulations show that surface-heating-induced thermal plumes generate strong near-ground horizontal inflow and coherent plume-merging structures, producing pedestrian-level convergence velocities of approximately 1–2 m/s, which is comparable to ventilation induced by moderate background winds.

Third, the CFD framework is applied to assess traffic-related pollutant dispersion at the neighborhood scale. Results indicate that buoyancy-driven ventilation substantially enhances pollutant removal under calm and light-wind conditions. Interactions between weak background winds and rising thermal plumes induce oscillatory flow structures and enhanced turbulence, effectively reducing near-surface pollutant accumulation.

Finally, drawing on a large ensemble of LES results, a parameterization scheme for urban ventilation under light-wind conditions is developed and incorporated into the UT&C model. By explicitly accounting for buoyancy intensity and urban morphology, the new scheme improves the representation of air exchange velocity.

This improvement directly enhances the assessment of heat and air quality risks in dense urban areas under light-wind and extreme-heat conditions, thereby providing a more robust scientific basis for urban design, planning, and climate-resilience strategies.

How to cite: Mei, S., Hu, S., and Sun, T.: Urban Ventilation in Light-Wind Conditions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1768, https://doi.org/10.5194/egusphere-egu26-1768, 2026.

The share of carbon emissions in the transport sector has been increasing year by year, and how to optimise the urban environment in order to promote green and low-carbon travel for residents has become a research hotspot. Much of the existing research has focused on the environmental characteristics of trip origins and destinations, with less attention paid to the impacts of the built environment in the travel path. This study takes Shenzhen, a megacity in China, as a case study to investigate the impact of street environment characteristics on residents' green travel behavior to urban parks. First, we conducted a questionnaire survey among visitors to urban parks between March and May 2023, finally collecting a total of 3,970 questionnaires. Then, by extracting and analyzing 137,000 street view images, we extracted street characteristics such as the green view index, sky openness index, sidewalk proportion, and wall coverage on respondent’s traveling road to urban parks. These street features were combined with visitor’s socio-demographic data, urban park’s characteristics, and other urban built environment to construct a generalized ordered logistic regression model. The results indicate that street greenery and sky openness are key factors contributing to low-carbon travel (Std=-2.886, p=0.000***; Std=-2.249, p=0.004***). In 2023, the total visitor volume to 176 urban parks in Shenzhen reached approximately 492 million visits, generating a total travel-related carbon emission of about 41,300 tons. The carbon emissions exhibited significant spatial variations, with higher emissions observed in coastal areas such as Nanshan District and Futian District. Additionally, there was a decreasing trend in carbon emission intensity from west to east. Based on the findings from travel mechanism studies, we proposed three different scenarios of low carbon development, including scenario of transportation system optimization with Shenzhen's public transport modal share reaching 65%, scenario of energy efficiency improvement with new energy vehicles accounting for 40% of the fleet, and scenario of street environment enhancement with the green visibility increased to 0.18. It found that these three scenarios would contribute to carbon emission reduction by 27%, 17%, and 4%, respectively. Even if the improvement of the street built environment does not provide the highest carbon emission reduction, it still has high potential for low-carbon development in high-density populated cities. This study reveals the critical role of the built street environment in promoting low-carbon travel and provides new methods and empirical support for low-carbon urban planning. Additionally, through future scenario analysis, this research offers scientific evidence for developing adaptive policies aimed at reducing carbon emissions.

How to cite: Zhang, W. and Guan, H.: How urban street-scape visual features influence carbon emissions from residents visiting urban parks: A case study of Shenzhen, China, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2060, https://doi.org/10.5194/egusphere-egu26-2060, 2026.

In high-density built-up areas, a key sustainability challenge is the spatial mismatch between ecosystem service (ES) supply and residents’ daily activity demand. Focusing on Longgang District (Shenzhen, China), we develop a reproducible workflow to track the structural evolution of ecosystem service value (ESV) and diagnose ES supply–demand mismatch from 2010 to 2023. We estimate ESV for five benchmark years (2010/2013/2016/2019/2023) and derive a residents’ activity intensity (RAI) index from multi-source digital proxies, including POI density, road-network node density, public-transport accessibility, and night-time light brightness. All indicators are standardised and integrated using a weighted overlay approach.

To characterise mismatch patterns, we apply an ESV–RAI two-dimensional coupling framework that uses district-wide means as thresholds and classifies spatial units into four coupled types (high/low ESV × high/low RAI). Results indicate a pronounced structural transition characterised by “low-value expansion and mid-value collapse”: the share of low-ESV areas increases from ~52% (2010) to nearly 59% (2023), while the mid-value layer—functioning as an intermediate transmission layer for ES delivery—contracts sharply, with an inflection around 2019. Low-ESV–high-RAI areas become the dominant coupled type, suggesting persistent structural barriers to translating ecological value into residents’ everyday living spaces.

Finally, we interpret corridor-based mechanisms through a hierarchical “urban–landscape coexistence” corridor system comprising three levels: regional ecological skeleton corridors, built-up transition corridors, and fine-grained embedded corridors supporting daily mobility and recreation. We argue that coordinated optimisation across this corridor hierarchy is critical to rebuild the intermediate transmission layer and mitigate ES–activity spatial mismatch in complex high-density cities.

How to cite: Cui, T.: Rebuilding the “intermediate transmission layer” of ecosystem services in a high-density city: ESV–RAI coupling and hierarchical urban–landscape coexisting corridors in Longgang (Shenzhen), 2010–2023  , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2188, https://doi.org/10.5194/egusphere-egu26-2188, 2026.

The urbanized Weather Research and Forecasting (uWRF) model is widely used for high-resolution urban climate modeling, yet its excessive computational cost restricts real-time forecasting and long-term climate assessment. To overcome this bottleneck, we propose AI-uWRF, a novel physics-informed generative emulator designed to bypass the computational demands of dynamical downscaling. The core architecture is a Hybrid Spatiotemporal Conditional Diffusion Model that integrates a Spatial Transformer within a U-Net backbone. A key innovation is the dual-stream condition encoder, which effectively fuses static urban surface heterogeneity (e.g., land use, topography) with dynamic large-scale atmospheric forcing. Unlike purely data-driven approaches, AI-uWRF incorporates physical constraints, including hydrostatic balance and continuity equations, into the training process to ensure thermodynamically consistent outputs. Validated against high-resolution (333 m) uWRF simulations in Wuhan, China, our emulator accelerates the generation of key meteorological fields (e.g., 2m temperature, 10m wind, surface pressure) by three orders of magnitude. The results demonstrate that AI-uWRF captures complex urban land-atmosphere interactions with high fidelity, offering a transformative tool for time-sensitive applications such as building energy optimization and probabilistic heatwave risk management.

How to cite: Song, J. and Zhang, Q.: AI-uWRF: A Physics-Informed Spatiotemporal Diffusion Transformer for High-Resolution Urban Weather Emulation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2266, https://doi.org/10.5194/egusphere-egu26-2266, 2026.

 
The precise identification of the "Production-Living-Ecological" spaces (PLES) plays a crucial role in  optimizing urban functional zones, constructing livable cities, and promoting balanced urban-rural development.  However, present studies on the functional identification of PLES exhibit a deficiency in comprehensive understanding and application of quantitative methods that integrate and interact with spatial elements. It is urgent to integrate multi-source geographical big data, considering the functional characteristics of different urban-rural regional systems, to establish a coherent and effective scheme for identifying spatial functions. To address this need, this study established three indices—Spatial Function Strength index (SFS), Spatial Function Coverage  index (SFC), and Spatial Function Interaction index (SFI) —from Point of Interest (POI), land cover, and mobile communication record, respectively. Utilizing road networks as the basic spatial unit for analysis, a decision tree was constructed for interpretation. Furthermore, landscape pattern indices were employed to analyze the spatialfunction characteristics at multiple scales including landscape, class and patch scale. The findings revealed significant functional disparities across various urban-rural systems. As increasing urbanization intensifies, there is an observed increase in spatial type diversity whereas the aggregation index of similar space decrease, along with the increase of shape complexity and patch density. The analysis identifies 13 distinct PLES patterns, notably,   ecological spaces predominantly occupy rural areas, while living spaces are primarily urban. The morphology and  distribution of production spaces vary with the dominant industries in different urban-rural systems. Fusion spaces  generally mirror the pattern of adjacent spaces, whereas interaction spaces are chiefly found in the transition zones  between urban and rural areas. Additionally, landscape pattern indices at the patch scale provide additional  evidence supporting systematic principles governing PLES from a more refined perspective. This study also  highlights those specific areas characterized by high spatial diversity but low agglomeration, providing new  scientific guidance for urban spatial planning and management.

How to cite: Liu, X. and Ma, S.: Spatial identification  of "production living ecological" spaces in urban-rural regional system by integrating multiple source data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3340, https://doi.org/10.5194/egusphere-egu26-3340, 2026.

EGU26-3673 | ECS | Posters on site | ITS3.12/NP8.8

Improving urban wind-flow prediction in complex built environments using a Cut-cell Cartesian grid CFD model 

Hyeon-Jong Lee, Jae-Jin Kim, and Hyun-Woo Cha

Abstract

This research explores the implementation of a Cut-Cell Method (CCM) within a Cartesian-grid CFD framework to mitigate the geometric distortions of building boundaries not aligned with the grid. By avoiding excessive grid refinement, CCM offers an efficient alternative for high-fidelity urban wind modeling. Performance was validated against AIJ wind-tunnel experimental data for Niigata, covering 80 points across 16 inflow directions. Comparisons with the conventional Stair-Step Method (SSM) demonstrate that CCM significantly enhances prediction accuracy. Quantitatively, the domain-averaged Index of Agreement increased by 18%, while RMSE and Mean Bias decreased by 18% and 55%, respectively. Detailed analysis reveals that while SSM creates artificial eddies and constricts street canyons, CCM more realistically captures building corners and spacing. However, in convergence and reattachment zones near tall and mid-rise buildings, CCM tends to overpredict reattachment lengths and enlarge secondary vortices, leading to localized wind speed underestimation. Despite these specific deviations, the method successfully brings all evaluated statistical indicators within recommended ranges. Overall, CCM provides a superior representation of complex urban morphology, proving essential for urban ventilation assessment, wind-corridor planning, and pollutant dispersion analysis. Future research should further evaluate this method under thermally stratified conditions to broaden its practical applicability.

 

Acknowledgments

This study was carried out with the support of 'R&D Program for Forest Science Technology '(Project No. "RS-2025-25404070")' provided by Korea Forest Service(Korea Forestry Promotion Institute).

Key words: CFD model, AIJ wind tunnel validation, cut-cell method, stair-step method

 

How to cite: Lee, H.-J., Kim, J.-J., and Cha, H.-W.: Improving urban wind-flow prediction in complex built environments using a Cut-cell Cartesian grid CFD model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3673, https://doi.org/10.5194/egusphere-egu26-3673, 2026.

EGU26-3687 | ECS | Posters on site | ITS3.12/NP8.8

A coupled CFD–Microphysics parameterization framework for urban-scale microclimate simulation 

Hyeonji Lee, Jang-Woon Wang, Jihoon Shin, Ye-seung Do, and Jae‒Jin Kim

Urban heat stress is governed by apparent temperature, yet many building-resolving CFD studies oversimplify humidity or impose it through external forcing. We develop a building-resolving CFD system with an online warm-phase microphysics coupling to simulate meter-scale wind–temperature–moisture variability in dense urban form. The model is applied to Jungnang-gu, Seoul (17–28 March 2024) and evaluated against hourly AWS 409 observations using MAE, RMSE, R², and 3D diagnostics. Relative to LDAPS, it better captures the temporal evolution of near-surface thermodynamic conditions, with RMSE = 1.17 °C for air temperature and 7.4% for relative humidity, and improves wind performance. Precipitation timing and variability are reproduced, though some hours show intensity bias, consistent with point-to-grid representativeness gaps and sensitivity to terminal-velocity assumptions. During rainfall, surface rain rate follows rainwater mass flux set by rain mixing ratio and net downward motion, and weak rain exhibits strong sub-kilometer intermittency. Urban ventilation structures shape coupled heat–moisture contrasts, producing hot–dry pockets under stagnation and cooler, moister conditions along ventilated corridors. These contrasts yield ~2–5 °C apparent-temperature differences over short distances, underscoring that heat-stress assessment should consider ventilation and humidity variability in addition to temperature.

 

Acknowledgments

This study was carried out with the support of 'R&D Program for Forest Science Technology '(Project No. "RS-2025-25404070")' provided by Korea Forest Service (Korea Forestry Promotion Institute).

 

Key words: Urban microclimate; CFD model; Warm-phase cloud microphysics; Humidity variability; Apparent temperature

How to cite: Lee, H., Wang, J.-W., Shin, J., Do, Y., and Kim, J.: A coupled CFD–Microphysics parameterization framework for urban-scale microclimate simulation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3687, https://doi.org/10.5194/egusphere-egu26-3687, 2026.

Industrial activity is among the principal sources of atmospheric emissions in urban areas. The ceramic industry, for example, emits high quantities of atmospheric contaminants, including particulate matter produced during clay extraction and production. The Santa Gertrudes ceramic industrial hub (SGCIH), located in the state of São Paulo, Brazil, is the sixth largest exporter of ceramic products in the world. The aim of this research is to present preliminary results concerning the effects of SGCIH ceramic industry agglomeration on the spatial distribution of particulate matter (PM10) in cities located in surrounding areas. In addition to the Santa Gertrudes (23,192 inhabitants; 48 ceramic industries in 2025) and Rio Claro (210,323 inhabitants; 18 industries), which are cities located in the SGCIH, we also analyzed PM10 data from four cities located far from the SGCIH, which have smaller numbers of ceramic industries: Piracicaba (440,835 inhabitants; 4 industries), Limeira (301,292 inhabitants; 2 industries), Americana (246,665 inhabitants; 1 industry), and Paulinia (116,674 inhabitants; 1 industry). Daily PM10 data from August 1, 2025, to September 30, 2025, obtained from six air quality monitoring stations located in the aforementioned cities, were used. PM10 medians were calculated and subsequently spatially interpolated using the inverse distance weighting algorithm. A first-degree trend surface map and a spatial autocorrelation pollutant map generated by the Getis‒Ord Gi statistical method were produced. The results revealed that the median PM10 was significantly greater in Santa Gertrudes (86 µg/m3) (p-value<0.001) than in Rio Claro (57 µg/m3), Limeira (47 µg/m3), Piracicaba (42 µg/m3), Americana (41 µg/m3) and Paulinia (32 µg/m3). Municipalities with a greater number of ceramic industries presented the highest concentration of PM10 (r=0.928; p-value=0.004). No significant association was observed between city population quantity and PM10 concentration (r=-0.257; p-value=0.718). These results may indicate that the effect of the number of ceramic industries on PM10 may be more important than city size is. The PM10 regional trend surface showed a slope toward the south-southeast, with the highest positive residual values of PM10 in the cities of the SGCIH and negative residual values in Americana and Paulinia, which were 34 km and 52 km from Santa Gertrudes, respectively. The spatial autocorrelation map revealed that PM10 presented a significant spatial autocorrelation index (z=1.874; p=0.039), with high PM10 values clustered ​​up to a 20-km radius around the SGCIH. We concluded that particulate matter  (PM10) in the atmosphere of the studied area presented a strong and positive spatial autocorrelation, which was influenced by the SGCIH location. We also reported that the PM10 concentration increases significantly with increasing proximity to the SGCIH. Moreover, compared with smaller cities, such as Santa Gertrudes and Rio Claro, which are located within SGCIH, populous cities located farther from the SGCIH presented lower PM10 concentrations. In the next step of this research, we will apply this spatial analysis methodology to evaluate the possible regional dispersion of MP10 and MP2.5 pollution using longer historical data series and a greater number of cities.

How to cite: Ferreira, M.: Spatial Analysis of Particulate Matter  (PM10) Air Pollution in Cities Surrounding a Ceramic Industrial Hub in the State of São Paulo, Brazil, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4583, https://doi.org/10.5194/egusphere-egu26-4583, 2026.

EGU26-4852 | ECS | Orals | ITS3.12/NP8.8

Multi-Scale Spatial Representation and Function–Structure Joint Optimization in Ports and Adjacent Areas 

Jin Sun, Yunzhuo Xu, Wenyuan Wang, and Zijian Guo

Focusing on ports as important infrastructure units within complex urban systems, this study addresses the challenges of highly coupled multifunctional land use, complex spatial structures, and scale-sensitive modelling in port and port-adjacent areas by developing an integrated framework for multi-scale spatial representation and function–structure joint modelling. First, considering the relatively limited spatial extent of port areas and the high requirements for spatial information accuracy, land-use functional characteristics are described from the perspectives of composition, morphology, and spatial pattern. A two-level spatial scale selection model is proposed, in which landscape indices combined with mean change-point analysis are used to determine appropriate spatial representation scales for port land-use functions. On this basis, a joint optimisation model of land-use functions and spatial structure in port and port-adjacent areas is further developed. The model explicitly accounts for interactions among different land-use functions and spatial heterogeneity, and quantitatively optimises functional configurations and spatial structures by maximising a weighted objective of economic, ecological, and social benefits. Model validation based on case studies demonstrates that the proposed framework effectively captures the impacts of multifunctional coupling on overall system performance and reveals the pathways through which port subsystems influence urban spatial structure and environmental responses. The study provides a quantitative modelling approach to support the analysis and optimisation of key infrastructure subsystems within complex urban systems.

How to cite: Sun, J., Xu, Y., Wang, W., and Guo, Z.: Multi-Scale Spatial Representation and Function–Structure Joint Optimization in Ports and Adjacent Areas, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4852, https://doi.org/10.5194/egusphere-egu26-4852, 2026.

EGU26-5196 | ECS | Posters on site | ITS3.12/NP8.8

 Large-eddy simulations of typhoon-landfall gust generation in areas surrounding super high-rise buildings 

Dong-Hyeon Kim, Ju-Hwan Rho, Chung-Hui Lee, and Jae‒Jin Kim

This study examines how a high-rise building complex (HB) in the Haeundae District of Busan, South Korea influences nearby airflow structures and gust generation using the Parallelized Large-Eddy Simulation Model (PALM) Version 6.0. The simulations were validated by comparing modeled wind speeds with observations collected during the landfall of Typhoon Hinnamnor that impacted the Busan area. To examine the influence of building height, we conducted a set of scenario experiments in which HB height was modified from 0% to 75% of the actual height in 25% increments. The results indicate that increasing HB height strengthens downdrafts and enhances flow separation, which markedly elevates pedestrian-level mean wind speeds and turbulent wind speeds. Meanwhile, the gust factor decreases as HB height increases, implying that gust factor alone is insufficient for representing gust intensity under strong-wind conditions. To compensate for this limitation, we conducted an additional analysis centered on turbulent gusts, showing that gust intensity rises in densely built low-rise areas adjacent to HB as HB height increases. Gust probability analysis further suggests that extreme gust events were very rare during typhoon landfall; however, with greater HB height, the occurrence of moderate and strong gusts increases in regions where flow separation is intensified. Overall, these results advance the understanding of airflow structures around high-rise buildings and demonstrate that high-resolution Large-Eddy Simulation under extreme weather conditions can improve wind hazard assessment accuracy and support evidence-based decisions for pedestrian safety and urban resilience.

 

Keywords: Large-eddy simulation; CFD model; High-rise building; Gust; Typhoon landfall

How to cite: Kim, D.-H., Rho, J.-H., Lee, C.-H., and Kim, J.:  Large-eddy simulations of typhoon-landfall gust generation in areas surrounding super high-rise buildings, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5196, https://doi.org/10.5194/egusphere-egu26-5196, 2026.

Cities are complex, multi-scale systems where the built environment, urban microclimate, and human behavior interact dynamically. Among these interactions, the response of building energy demand to extreme heat is a critical feedback loop that impacts urban functional stability and energy security. However, quantifying these cross-sectoral feedbacks—specifically how outdoor thermal variations translate into indoor cooling behavior and energy demand—remains a significant modeling challenge. To address this, we propose a hybrid modeling framework that integrates machine learning with a physics-based building energy balance model to bridge the gap between urban microclimate and building energy consumption. Our approach estimates the power consumption of air conditioning (AC) systems by distinguishing operational states based on the coupling and decoupling of indoor and outdoor climate variations. The framework employs an XGBoost model to identify AC operation within optimal time windows, followed by the Pelt algorithm to detect state transition points and pinpoint exact operational periods. Subsequently, a Resistance-Capacitance (R-C) model is parametrized using coupled indoor-outdoor climate data during AC-off periods, which is then utilized to estimate real-time AC power.

The model was validated against data from a residential building in Beijing, demonstrating good accuracy in both predicting AC operating status and estimating power loads. The hybrid model was then applied to real-world urban scenarios to quantify the impact of extreme heat on cooling demand using only monitored climate variations, independent of direct energy metering data. This research provides a robust quantitative tool for climate-adaptive planning, advancing our ability to model the complex dependencies between urban energy systems and a changing climate.

How to cite: Cao, Z. and Kai, W.: Impact of extreme heat on building cooling energy demand: a hybrid model based on the coupling of indoor and outdoor climate variations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5301, https://doi.org/10.5194/egusphere-egu26-5301, 2026.

Understanding the interactions between competing land policies is crucial for identifying governance challenges and assisting urban planners and policy analysts in make informed decisions. However, a methodology for incorporating land use patterns and the policy implementation processes within the framework of hierarchical land management remains underexplored. Here, we employ an agent-based model (ABM) to investigate how land use change occurs as policies intersect across different hierarchical levels and branches of government in Wuhan, China. Changes in land use arise from the interplay between five agents—the central level, the local level that incorporates three departments, and the village collective level—in the decisions on land acquisition, conversion, and reclamation. Four parameters characterize the enforcement levels of relevant policies, and multi-objective optimization with genetic algorithms was applied to calibrate them. The results show that: (1) Our ABM exhibits a figure of merit value of 0.3 at the city level and 0.58 in the larger urban area, indicating its capability to simulate real land use dynamics. (2) Policy implementation gaps led to high land conversion and low farmland reclamation. (3) The dynamic enforcement scenarios provide a viable pathway for negotiated governance, enabling demand-responsive rate attenuation and conflict mitigation, which is distinct from the exacerbated land use conflicts observed under the other scenarios. (4) Policy should incorporate adaptive mechanisms to maintain a buffer between competing land demands rather than binary constraints. This ABM introduces a novel hierarchical framework to decode policy interplay and implementation tensions, advancing sustainable land governance and urban planning insights.

How to cite: Gao, J.: How Do Interacting Policies Reshape Land Use Patterns? A Hierarchical, Cross-Departmental Agent-Based Exploration, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5353, https://doi.org/10.5194/egusphere-egu26-5353, 2026.

Urban agglomerations function as integrated spatial systems in which infrastructure provision and public services jointly shape urban livability outcomes. While existing studies largely focus on individual cities, empirical evidence at the urban agglomeration scale remains limited. Addressing this gap, this study examines disparities in livability across major Chinese urban agglomerations from an integrated infrastructure and public service perspective.

Using multi-source statistical data covering multiple urban agglomerations in China, a comprehensive indicator system is constructed to capture transportation infrastructure, public green spaces, cultural facilities, and public service provision. Principal component analysis (PCA) and factor analysis are employed to extract key dimensions influencing livability, followed by cluster analysis to classify urban agglomerations based on their infrastructure structure and livability performance.

The results reveal pronounced heterogeneity in the capacity of infrastructure to support livability across urban agglomerations. Transportation infrastructure, measured by road network length, exerts a stronger influence on livability in rapidly expanding and spatially dispersed agglomerations, whereas public green spaces, cultural facilities, and public service facilities play a more prominent role in relatively mature and compact agglomerations. Based on these differentiated effects, urban agglomerations can be broadly categorized into two dominant types: transportation-oriented agglomerations, where mobility-oriented infrastructure constitutes the primary livability foundation, and ecology-oriented agglomerations, where green spaces, environmental quality, and public service provision contribute more substantially to livability enhancement.

By integrating infrastructure and public services into a unified analytical framework at the urban agglomeration scale, this study extends the empirical understanding of livability formation mechanisms beyond the city level. The findings offer policy-relevant insights for differentiated infrastructure and public service strategies, emphasizing the importance of aligning development priorities with the structural characteristics and developmental stages of urban agglomerations.

How to cite: jing, S. and zhao, H.: Spatial Disparities in Livability across Chinese Urban Agglomerations:An Infrastructure and Public Service Perspective, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6127, https://doi.org/10.5194/egusphere-egu26-6127, 2026.

Cities are complex multi-scale systems in which transport networks interact dynamically with the built environment, such as population distribution, land use, and transport network structure, leading to traffic congestion patterns that vary across space and time. Considering the complex and dynamic characteristics of traffic congestion, it is essential to explore the spatiotemporal heterogeneity and dynamics in the relationships between built environment factors and urban traffic congestion to develop effective policies that enhances urban livability. Hence, this study employs a geographically weighted machine learning framework that integrates random forest (RF) with geographic weighted regression (GWR), referred to as the geographically weighted random forest (GWRF). Additionally, the SHapley Additive exPlanations (SHAP) method is applied to identify dominant associated factors, interpret nonlinear relationships, and reveal local feature differences between explanatory variables and traffic congestion across different time periods. An empirical case study is conducted in Chongqing, China, a mountainous megacity characterized by complex transport dynamics and strong spatial constraints. The case study utilizes multi-source datasets collected over five months, selects 25 candidate variables that represent built environment characteristics, including land-use diversity, road network design, public transit service, and destination accessibility, as well as demographic and socioeconomic attributes, such as population density and economic indicators. Traffic congestion patterns are examined during morning and evening peak hours on both weekdays and weekends to capture temporal dynamics. Compared with traditional spatial regression models and global machine learning approaches, the geographically weighted machine learning framework achieves about 15-20% higher predictive accuracy. Moreover, the framework exhibits improved stability and adaptability by explicitly incorporating a spatial weighting matrix. From a global perspective, betweenness centrality, office density, bus stop coverage, and shopping density are identified as the dominant factors associated with traffic congestion across the four peak periods. The above results further reveal the nonlinear associations, and threshold effects between key explanatory variables and congestion levels. From a local perspective, the impacts of dominant factors display strong spatial clustering, with the pattern, magnitude, and direction of these associations varying significantly across different spatial regions and time periods. Overall, these findings enhance the understanding of urban transport dynamics, and provide valuable insights for urban planners and operators in developing the planning and management strategies to alleviate traffic congestion and improve urban livability. 

How to cite: Chen, S., Qin, S., and Wang, W.: Exploring spatiotemporal heterogeneity and dynamics of the built environment impacts on urban traffic congestion with geographically weighted machine learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7329, https://doi.org/10.5194/egusphere-egu26-7329, 2026.

EGU26-7380 | ECS | Orals | ITS3.12/NP8.8

A High-Quality Daily Nighttime Light Dataset for Dynamic Urban Sensing 

Zixuan Pei, Xiaolin Zhu, Yang Hu, Jin Chen, and Xiaoyue Tan

Nighttime light (NTL) data at daily scales presents an innovative foundation for monitoring human activities, offering vast potential across various research domains such as urban planning and management, disaster monitoring, and energy consumption. The daily moonlight-adjusted nighttime lights product (VNP46A2), sourced from Suomi National Polar-orbiting Partnership Visible Infrared Imaging Radiometer Suite (NPP-VIIRS), has been providing globally corrected daily NTL data since 2012. However, persistent challenges, such as fluctuations in the daily NTL series due to spatial mismatch and angular effects, as well as data holes, have significantly impacted the accuracy and comprehensiveness of extracting daily NTL changes. To address these challenges, a dataset production framework focusing on error correction, interpolation, and validation was developed. This framework led to the creation of a high-quality daily NTL (HDNTL) dataset from 2012 to 2024, which specifically targets 653 cities with populations predictably exceeding one million in 2025. A comparative analysis with the VNP46A2 dataset revealed promising results in spatial mismatch correction for two sample areas – the airport and highway (angular effect can be ignored). These areas exhibited reduced fluctuations in HDNTL time series and enhanced spatial consistency among pixels with homogeneous light sources. Furthermore, the correction of angular effects across various urban building landscapes demonstrated sound improvements, mitigating angular effects in different directions and reducing periodicity from the angular impacts. The spatiotemporal interpolation of data holes shows high similarity with reference data, as indicated by a Pearson correlation coefficient (r) of 0.99, and it increased the valid pixels of all cities by about 2 %. The HDNTL dataset exhibited enhanced consistency with high-resolution Sustainable Development Science Satellite 1 (SDGSAT-1) NTL data regarding the NTL change rate. Also, it showed high alignment with ground truth data of power outages, showcasing superior performance in short-event detection. Overall, the HDNTL dataset effectively mitigates instability in daily series caused by spatial mismatch and angular effects observed in VNP46A2, improving data comparability across both time and space. This dataset enhances the ability of the NTL to reflect the ground events, providing a more accurate reference for daily-scale nighttime light research. Additionally, the dataset production framework facilitates easy updates from future VNP46A2 products to HDNTL. The HDNTL is openly available at https://doi.org/10.5281/zenodo.17079409 (Pei et al., 2025). This study was supported by the National Natural Science Foundation of China (no. 42401474).

How to cite: Pei, Z., Zhu, X., Hu, Y., Chen, J., and Tan, X.: A High-Quality Daily Nighttime Light Dataset for Dynamic Urban Sensing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7380, https://doi.org/10.5194/egusphere-egu26-7380, 2026.

Nighttime light (NTL) data, a remote-sensing record of surface brightness, offer unique observations of cities. With the advantage of high spatiotemporal coverage, NTL data have been widely used to extract urban extents, monitor human activities, quantify socio-economic resources, and estimate energy consumption. Recent products with a higher spatiotemporal resolution have further expanded applications, enabling daily 500-m-resolution monitoring of festivals, wars, and fishing vessels. Most existing studies, however, use only the radiance or spatial extent of NTL and ignore the angular information, which limits their application in observing the internal spatial structure of cities.

Beyond brightness features, the angular information of NTL data characterizes the urban spatial structure. As the viewing zenith angle (VZA) of daily satellites varies, recorded radiance differs because buildings increasingly mask the light, creating an angular effect. Existing studies have modelled angular effects with linear, quadratic, or polynomial models, revealing divergent angular signatures between urban centres and suburbs. However, two gaps persist. First, no unified angular-effect model exists. Although linear and quadratic regressions can depict positive, negative, or U-shaped angular effects, the angular effects they quantify are not directly comparable. Second, explanatory insight into the drivers of the angular effects remains unclear. Although correlations with building height and density have been reported, interpretability is lacking. These knowledge gaps hinder the translation of angular effect research from theory into practice.

Here, we quantify and explain the angular effects across five U.S. cities—Baltimore, Boston, Dallas, Washington D.C., and New York—from 2013 to 2024. We first construct a novel model that captures the relationship between VZA and NTL intensity, introducing a new metric for quantifying angular effects. The model performs well overall, with R2 > 0.6 for more than 70% of pixels. We then develop a series of indicators and apply an interpretable machine-learning framework. We found that pixels with high angular-effect values are characterized by high building-light blockage, high building density and significant variation in building height. All ten indicators collectively explain the angular effect. This study bridges the gap between the angular effects and urban structure, enabling large-scale and high-frequency monitoring of urban structure in data-deficient regions (such as Africa) in the future.

How to cite: Li, S., Chen, W., and Zhou, Y.: Modelling Multi-angle Nighttime Light Observations to Investigate the Impact of Urban Structure on Angular Effect, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9121, https://doi.org/10.5194/egusphere-egu26-9121, 2026.

EGU26-9182 | Posters on site | ITS3.12/NP8.8

Risk Assessment of Bridges and Analysis of Road Traffic Scenarios through Traffic Simulation 

Epameinondas Lyros, Spyros Barkas, and Athanasios Theofilatos

This study focuses on bridge risk assessment and the analysis of alternative road network scenarios by using traffic simulation methods. The primary objective of the research is to assess the risk associated with the Neochori–Katochi Bridge and to analyze alternative road network scenarios in the event of partial or total loss of its serviceability, particularly due to seismic events. The bridge is located at the Municipality of the Sacred City of Messolonghi, in the Regional Unit of Aetolia-Acarnania, western Greece, and constitutes a critical link in the local and regional road network. The study area corresponds to the expanded Municipality, with approximately 32,000 inhabitants, comprising the municipal units of Messolonghi,
Aitoliko and Oiniades. The Oiniades unit, with about 9,000 inhabitants, hosts the Neochori–Katochi Bridge, which lies along a provincial road and serves as a key connection for daily commuting, freight transport and regional accessibility. The bridge has an approximate length of 190 m and is located at coordinates 38.4094° N, 21.2605° E. Given its strategic importance, any disruption would have significant social and economic impacts to the wider area. To address these issues, an integrated methodological framework was applied, combining seismic, traffic and behavioural analyses. Data collection included traffic flows, speeds and geometric characteristics of the road network, as well as structural and seismic information related to the
bridge. In parallel, a questionnaire-based survey was conducted among residents and drivers of the surrounding areas to capture travel behaviour and route choice preferences under both normal and disrupted traffic conditions. Based on seismic hazard maps previously developed for the study area, our analysis evaluates the seismic risk and functional importance of the bridge. Secondly, multiple traffic management and network reconfiguration scenarios are developed to represent potential conditions after loss of bridge serviceability. These scenarios include alternative routing strategies designed to accommodate displaced traffic flows while minimizing traffic congestion and travel delays. Traffic microsimulation models are
used to analyse and compare the proposed scenarios. The evaluation focuses on key performance indicators such as volume to capacity ratios (v/c) and travel delays. Specific attention is given to the ability of the surrounding road network to absorb rerouted traffic without severe degradation of operational conditions. Moreover, the questionnaire survey data are analysed using discrete choice models, in order to identify the factors that influence drivers’ selection of alternative routes. Variables such as travel time, perceived safety, reliability and road characteristics are examined
to understand how users adapt their behaviour in response to local network disruptions. Overall, the current research offers a comprehensive approach to bridge risk assessment that goes beyond structural considerations by focusing on traffic performance and road users’ behaviour. The findings support the development of more resilient road network planning strategies and could assist in practical guidance for emergency traffic management and long-term infrastructure improvement in seismically active regions.

How to cite: Lyros, E., Barkas, S., and Theofilatos, A.: Risk Assessment of Bridges and Analysis of Road Traffic Scenarios through Traffic Simulation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9182, https://doi.org/10.5194/egusphere-egu26-9182, 2026.

EGU26-9395 * | Orals | ITS3.12/NP8.8 | Highlight

Impacts of Urban Vegetation on Cooling Energy Demand Across 100 Global Cities 

Xizhu He, Naika Meili, and Simone Fatichi

Urban trees are widely promoted to mitigate urban heat and reduce cooling demand through shading and evapotranspiration. However, added moisture can increase dehumidification energy loads, making the net impact of greening on building energy demand climate-dependent and poorly quantified. Here, we use the Urban Tethys-Chloris model coupled with a Building Energy Model (UT&C-BEM) to quantify vegetation-driven impacts on summer air-conditioning energy consumption (ECAC,summer) in 100 globally significant cities spanning diverse climates, urban forms, and vegetation patterns. Under present-day vegetation cover, urban trees reduce mean daily summer cooling energy demand in all 100 cities, but with a clear trade-off between absolute energy savings and relative sensitivity of savings to green area. By systematically increasing tree fraction from each city’s baseline up to 100% cover, we found that greening efficiency is highest in hot arid cities and markedly weaker in hot humid climates, where enhanced dehumidification demand offsets sensible cooling benefits. Cities in hot arid climates, where greening efficiency is highest, should prioritize tree-based cooling as a cost-effective energy mitigation strategy.

How to cite: He, X., Meili, N., and Fatichi, S.: Impacts of Urban Vegetation on Cooling Energy Demand Across 100 Global Cities, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9395, https://doi.org/10.5194/egusphere-egu26-9395, 2026.

EGU26-10686 | ECS | Posters on site | ITS3.12/NP8.8

Evaluating tuberculosis service accessibility in Pakistan by analyzing population movement patterns from telecom mobility and survey data  

Oluwafemi John Ifejube, Christina Mergenthaler, Peter Stephens, Umar Saif, Yee Theng Ng, Bilal Butt, Rayi Syed, Frank Cobelens, and Ente Rood

Background

Geographic access to healthcare is considered in urban environments to aid strategic planning and evaluation of healthcare interventions. Evidence has shown that, in addition to geographic access, multiple factors influence the travel behavior of people seeking health services. Yet most studies have largely framed the issue from the perspective of how far people should travel, while few have explained how far people actually travel, thereby overlooking potential insights into travel behaviors.

Methods

In this research, we used in-person interviews, telecom mobility data, and spatial analysis to estimate people’s accessibility to TB service points in Pakistan. Characteristics of TB service points, including urbanicity, socio-economic class, and administrative province, were further analysed for their association with TB service accessibility. We compared the accessibility rates obtained from in-person interviews among people visiting TB service points with telecom mobility data to assess whether measured population movements to TB service points differ by data source.

Results

Our results show that significant variations in TB service accessibility are associated with administrative provinces, and the density of TB service points. We found a significant difference between the geographic accessibility measured by the two data sources across distance bands. We also found that relative, and not absolute, TB service accessibility is similar across both data sources, with a steeper decay curve in the interview data.

Conclusions

While telecom mobility data and survey data capture different population movement patterns, both provide insights which may help to align service availability with population needs and improve the well-being of the population.

How to cite: Ifejube, O. J., Mergenthaler, C., Stephens, P., Saif, U., Ng, Y. T., Butt, B., Syed, R., Cobelens, F., and Rood, E.: Evaluating tuberculosis service accessibility in Pakistan by analyzing population movement patterns from telecom mobility and survey data , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10686, https://doi.org/10.5194/egusphere-egu26-10686, 2026.

Global climate change driven by carbon dioxide (CO2) emissions has brought great challenges to countries around the world. Road transport takes an important part in CO2 emissions from transport sector. Although many studies have explored road transport CO2 emissions, few studies focused on CO2 emissions from both highway transport and urban road transport at city level. To address this gap, this study examines road passenger transport CO2 emissions across 31 provincial-level divisions and 325 cities in China using a bottom-up method, and analyzes their spatial-temporal characteristics and driving factors. The results show that road passenger transport CO2 emissions in China increased steadily from 2010 to 2023, with a compound annual growth rate of 9.20%. The overall spatial pattern is characterized by higher emissions in the eastern regions and lower emissions in the western regions. In addition, the city level CO2 emissions have significant spatial-temporal heterogeneity and disparities in CO2 emissions have narrowed over time. Globally driving factors analysis indicates the population size and economic development are key factors of CO2 emissions. At the city level, the effects of population, economy, road infrastructure, and land use on CO2 emissions exhibit spatial-temporal non-stationarity among cities, indicating dynamic changes in CO2 emission driving mechanisms across different periods and spaces. This study provides critical insights for policymakers aiming to reduce road transport CO2 emissions and achieve the objectives of carbon peaking and carbon neutrality.

How to cite: Qin, S., Chen, S., and Wang, W.: Spatial-temporal characteristics and driving factors of city level CO2 emissions from road passenger transport in China, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12565, https://doi.org/10.5194/egusphere-egu26-12565, 2026.

Compounding with global warming induced by carbon emissions, urbanization is exerting an additional warming effect, further threatening local urban residents. However, due to the heterogeneity within urban areas, the risk among residents in the same city varies significantly. Researchers have explored various methods to describe urban surfaces, among which the Local Climate Zone (LCZ) framework has proven to be an effective tool for characterizing diverse urban morphologies globally. Although global LCZ mapping products are available, inter-annually comparable LCZ time series remain scarce in the current literature. Additionally, the evaluation of thermal characteristics of urban morphology often relies on comparing median or average Land Surface Temperature (LST) between LCZ types, which can introduce substantial bias due to spatial autocorrelation caused by terrain differences, uneven human activities, and other factors. Thus, there is an urgent need for a dynamic monitoring and impact evaluation paradigm for urban morphology.

In this study, we present an annual LCZ time-series mapping framework and generate time series from 2000 to 2020 for three major Chinese urban agglomeration: Jingjinji, the Yangtze River Delta, and the Greater Bay Area. Comparing with baseline (supervised classification directly), LCZ time-series generated by our framework ensured the consistency between years. Furthermore, by integrating the LCZ time series proposed in this study with MODIS Land Surface Temperature (LST) datasets, we developed a time-series analysis method to quantify LST changes induced by different urban morphology transformations. The mapping results reveal that high-rise buildings are the primary distinguishing feature between urban areas of different sizes. Over the past two decades, the composition of urban morphology has been converging between urban areas of varying sizes but diverging within intra-city land use zones. Moreover, urban morphology patterns differ significantly between urban expansion areas and urban renewal areas. Our findings indicate that the impact of urban morphology changes varies significantly. Specifically, urban renewal, predominantly characterized by vertical development, exerts an asymmetric effect on urban temperatures: it mitigates urban warming during the day but intensifies it at night. In contrast, the effect of urban expansion on urban warming is more pronounced during the day than at night. At the city scale, changes in urban morphology generally contribute to a warming effect, both diurnally and nocturnally. Urban expansion is identified as the primary driver of rising city temperatures. However, the divergent impacts of vertical development, which is likely to dominate future urbanization, must not be underestimated.

How to cite: Zhao, J.: Mapping the Thermal Footprint of Urbanization: A Long-Term Perspective based on Local Climate Zone Dynamics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13029, https://doi.org/10.5194/egusphere-egu26-13029, 2026.

Urban areas are increasingly vulnerable to extreme thermal conditions due to rapid urbanization and climate change. The accurate prediction of ambient air temperature (AT) at fine temporal scales is essential for mitigating the impacts of urban heat waves, heat pockets, and heat islands. Despite ongoing research, limited interpretability of traditional AI models has constrained their utility in decision-making. This study aims to improve real-time temperature forecasting in the Central National Capital Region (Central-NCR) of India through explainable machine learning techniques. Hourly AT was modeled using four advanced machine learning algorithms—Random Forest (RF), Gradient Boosting (GB), XGBoost, and LightGBM (LGBM). A structured workflow was followed involving data preprocessing, hyperparameter tuning, cross-validation, model training, and evaluation. Model performance was compared using residual plots, validation curves, and statistical metrics including RMSE, MAE, MSE, R², MAPE, and Explained Variance Score (EVS). A Taylor dia-gram was used for holistic model comparison. Among all tested models, RF demonstrated the highest predictive accuracy, achieving an R² of 0.81 and the lowest RMSE of 3.36 during the test phase. Relative humidity (RH) and barometric pressure (BP) emerged as the most influential predictors. SHAP analysis further confirmed RH, BP, and solar radiation (SR) as key drivers of AT variability. Seasonal patterns indicated that increased RH during monsoon months reduced AT, while elevated SR levels during summer contributed to higher temperatures. Dependence and partial dependence plots revealed non-linear interactions: RH exhibited a strong inverse relationship with AT, SR drove exponential increases, and BP displayed oscillatory patterns reflective of atmospheric fluctuations. The integration of explainable AI techniques with meteorological data enables more accurate and interpretable urban temperature forecasting. These insights can support policymakers and urban planners in developing informed strategies for heat mitigation, regulatory compliance, and climate adaptation.

How to cite: Mahato, S.: Towards Climate-Resilient Cities: Exploring Meteorological Drivers of Urban Heat Variability with Explainable Machine Learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13542, https://doi.org/10.5194/egusphere-egu26-13542, 2026.

Rapid urban expansion in transitional regions intensifies interactions between human activities and ecological systems, yet quantitatively capturing the spatial balance between anthropogenic pressure and ecological capacity remains a major scientific challenge. Existing approaches often conceptualize human–environment interactions or focus on land-change outcomes without explicitly measuring coupling strength, direction, and spatial dynamics. This study introduces a quantitative geospatial analytics framework to assess human–environment coupling across space and time, using Prishtina (Kosovo) as a representative transitional urban system.

The framework conceptualizes the urban system through two spatially explicit and normalized gradients: an anthropogenic forcing gradient, representing cumulative human pressure, and a geo-ecological capacity gradient, capturing the environment’s ability to regulate and respond to that pressure. These gradients are derived from harmonized multi-source geospatial indicators, including satellite-based environmental proxies and complementary spatial datasets, and are integrated through standardized preprocessing, normalization, and data-driven weighting procedures to ensure spatial comparability and analytical robustness.

Human–environment coupling is quantified using a normalized spatial index ranging from 0 to 1, where higher values indicate balanced interactions and lower values signal increasing imbalance between anthropogenic forcing and ecological capacity. Spatial statistical techniques, including spatial autocorrelation and hotspot analysis, are applied to examine clustering patterns, transition zones, and emerging disequilibrium, while temporal analysis supports the exploration of coupling trajectories under rapid urban transformation.

The proposed framework enables spatially explicit investigation of human–environment coupling heterogeneity within Prishtina and supports the identification of zones characterized by balance, dominance, or transition. By integrating multi-source geospatial data with advanced geospatial analytics, the study offers a transferable quantitative approach for diagnosing human–environment interactions and informing sustainability-oriented spatial planning in transitional urban regions.

How to cite: Berila, A., Chassin, T., and Sulzer, W.: Spatial quantification of human–environment coupling using multi-source geospatial data and geospatial analytics: evidence from Prishtina, Kosovo, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15419, https://doi.org/10.5194/egusphere-egu26-15419, 2026.

EGU26-15824 | ECS | Orals | ITS3.12/NP8.8

Urban thermal environments as interconnected systems: Emergent causal networks and dynamic synchronization 

Chenghao Wang, Yihang Wang, Zhi-Hua Wang, and Xueli Yang

Urban heat is a growing concern, especially under global climate change and continuous urbanization. However, the understanding of its spatiotemporal propagation behaviors remains limited. In this study, we leverage a data-driven modelling framework that integrates causal inference, network topology analysis, and dynamic synchronization to investigate the structure and evolution of temperature-based causal networks across the continental United States. We perform the first systematic comparison of causal networks constructed using warm-season daytime and nighttime air temperature anomalies in urban and surrounding rural areas. Results suggest strong spatial coherence of network links, especially during nighttime, and small-world properties across all cases. In addition, urban heat dynamics becomes increasingly synchronized across cities over time, particularly for maximum air temperature. Different network centrality measures consistently identify the Great Lakes region as a key mediator for spreading and mediating heat perturbations. This system-level analysis provides new insights into the spatial organization and dynamic behaviors of urban heat in a changing climate.

How to cite: Wang, C., Wang, Y., Wang, Z.-H., and Yang, X.: Urban thermal environments as interconnected systems: Emergent causal networks and dynamic synchronization, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15824, https://doi.org/10.5194/egusphere-egu26-15824, 2026.

Accurate weather data are critical for simulating building energy use and assessing power-grid demand. Typical meteorological year (TMY3) datasets are widely used for this purpose but represent long-term average conditions assembled from different years, limiting their ability to capture interannual variability and extreme events that often drive peak loads. Actual meteorological year (AMY) data provide continuous, year-specific weather records and thus offer a more realistic depiction of variability and extremes. However, their application has been constrained by limited duration, spatial coverage, and the coarse resolution of many long-term products. In this study, we compare residential building energy consumption across more than 500 U.S. urban locations using TMY3 data and 23 years of AMY data enabled by the Historical Comprehensive Hourly Urban Weather Database (CHUWD-H v1.1). AMY-based simulations reveal substantial year-to-year variability and consistently higher peak loads than TMY3-based results. Relative to the 23-year AMY simulations, TMY3 underestimates cooling energy demand by 11.7 ± 7.5% and overestimates heating demand by 13.6 ± 16.5% on average. These findings demonstrate that reliance on TMY3 can systematically misrepresent both energy demand magnitude and extremes, and underscore the necessity of long-term, urban-resolved AMY datasets for robust building energy assessments and climate-resilient power-system planning.

How to cite: Leffel, J., Wang, C., and Horsey, H.: Reliance on typical weather data misrepresents cooling and heating energy use: Insights from 23 years of building energy simulations across the U.S., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16025, https://doi.org/10.5194/egusphere-egu26-16025, 2026.

This study aims to develop a high-resolution forecast–data assimilation cycling system to support Urban Air Mobility (UAM) operations. We implemented and evaluated a WRF-based 3DVAR–IAU (Incremental Analysis Update) cycling framework. Although 3DVAR is computationally efficient and suitable for high-frequency assimilation, directly incorporating the analysis into model integration can cause initial forecast discontinuities and spin-up issues. IAU mitigates these problems by gradually applying the analysis increment over the assimilation window.

The coupled WRF–WRFDA cycling procedure was automated to repeatedly perform 3DVAR analyses and subsequent forecasts using IAU. A preprocessing workflow was also established to process surface and vertical-profile observations, including LiDAR measurements, for data assimilation. To evaluate the performance of the system, we conducted two experiments: a CYCLE experiment (applying 3DVAR–IAU cycling) and a NOCYCLE experiment (a WRF-only free forecast without data assimilation). Forecast performance was assessed against observations using bias, root-mean-square error (RMSE), and correlation coefficients.

The results indicate that applying IAU reduces initial forecast discontinuities and leads to more stable early forecast behavior compared to NOCYCLE. Time–height cross-sections of wind speed error show that the CYCLE experiment generally produces smaller errors than NOCYCLE throughout the evaluation period. Consistently, the CYCLE experiment tends to yield lower RMSE and higher correlations relative to NOCYCLE for most vertical levels, indicating improved agreement with observations. Overall, these findings suggest that the proposed 3DVAR–IAU cycling approach can enhance the quality of assimilated initial conditions and contribute to continuous performance improvements in UAM-specific high-resolution prediction systems.

 

Key words: WRF, WRFDA, 3DVAR, IAU(Incremental Analysis Update), Cycling data assimilation

 

How to cite: Cho, S.-I. and Shin, J.: Performance Evaluation of a UAM-Specific High-Resolution Forecast-Data Assimilation Cycling System, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16621, https://doi.org/10.5194/egusphere-egu26-16621, 2026.

Despite being a key determinant of urban energy demand, anthropogenic heat emissions, and indirect carbon dioxide emissions, precise observational data for entire cities remains scarce. This study develops a data-driven framework that reconstructs monthly electricity consumption for individual parcels across Seoul by integrating building characteristics, microclimate, and human activity. We collected millions of monthly observation records from 2020 to 2024 and converted billed electricity quantities into electricity use intensity (EUI, kWh m⁻²) using building floor areas. These records were linked with parcel-level attributes (e.g., land use, land price, gross floor area, construction year), local climate zones, socioeconomic indicators, high-density Smart Seoul City Data of Things (S-DoT) meteorological observations, and hourly living population data. Random Forest and LightGBM models were trained and evaluated using 5-fold cross-validation. LightGBM demonstrated the best performance across all parcels, achieving a Mean Absolute Error (MAE) of 6,712 kWh, a Weighted Mean Absolute Percentage Error of 39.6%, and an R² of 0.709. SHAP (SHapley Additive exPlanations) analysis revealed urban land price, building size, construction year, and income as key determinants of EUI. Concurrently, the living population and microclimate variables exerted nonlinear additional effects, particularly in high-activity commercial districts. High-density, high-rise business centers exhibited high power intensity despite relatively mild outdoor maximum temperatures, suggesting a decoupling between indoor cooling demand and the surrounding thermal environment. The estimated dataset for building-specific electricity consumption across the entire city provides essential data for artificial heat estimation, energy planning, and future urban climate and emissions modeling.

How to cite: Lee, Y. and Im, J.: Citywide Parcel-Level Electricity Use Estimation from Building GIS, Microclimate, and Human Activity Data in Seoul, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17064, https://doi.org/10.5194/egusphere-egu26-17064, 2026.

EGU26-18030 | Posters on site | ITS3.12/NP8.8

Urban Geo-climate Footprint (UGF) for Classifying Italian Cities by Geological and Climatic Features 

Saverio Romeo, Mauro Bonasera, Maria Paola Campolunghi, Gianluigi Di Paola, Paolo Maria Guarino, Gabriele Leoni, Raffaele Proietti, and Francesco La Vigna

Urban areas are increasingly exposed to complex interactions of geological, climatic, and anthropogenic pressures. The UGF methodology (Lentini et al., 2024), already applied to more than 40 European cities, provides a structured approach to assess these multi-dimensional conditions and support urban planning and risk management. In this study, UGF was applied to 21 Italian regional capitals, selected to capture the geographic, climatic, and structural diversity of the country, from alpine regions to coastal plains and southern volcanic districts. Italy thus represents an ideal natural laboratory to test the methodology, offering a wide range of geological and climatic settings within a single country.

The methodology integrates multiple drivers: deep geological processes (DEE, e.g., seismicity and volcanism, gas emissions), superficial processes (SUP, e.g., landslides, subsidence, floods, coastal erosion), exogenous processes (EXO, e.g. heavy rains, droughts, sea level change), geological complexity (GEO, e.g., stratigraphy, groundwater, slope), and anthropogenic pressures (SAP, e.g., land use change, soil sealing, pollution). For each city, the UGF Index quantifies the intensity of these drivers, allowing classification into four UGF classes that reflect the spectrum of urban geo-climatic conditions.

Results from Italy highlight a wide range of situations: Trento and Campobasso fall into UGF-1, indicating minimal geologic-climatic pressures, while Napoli and Genova are classified as UGF-4 due to the combined influence of high-intensity drivers, including active volcanism, high seismicity, subsidence, and strong anthropogenic pressures. Intermediate classes (UGF-2 and UGF-3) include cities such as Milano, Firenze, Bari, and Venezia, where moderate interactions of these drivers prevail.

Geographical patterns emerge from the analysis of drivers. UGF index generally increases southward, reflecting higher exposure to Mediterranean climatic extremes, active seismicity along the Apennines, and southern volcanic districts. Coastal cities show high SUP and EXO contributions due to erosion, storm surges, and sea-level rise, while SAP is prominent in large urban centers, reflecting land consumption, groundwater contamination, and subsurface instability. The GEO driver is relatively consistent across the country, emphasizing Italy’s intrinsic geodiversity.

It is important to note that UGF classes do not rank cities by “risk” or “misfortune,” but rather identify the prevailing geological, climatic, and anthropogenic pressures to support planning and mitigation. A semi-qualitative assessment of geo-benefits further highlights positive contributions to urban systems, with cities such as Milano, Napoli, Palermo, Roma, Trento, Trieste, and Venezia showing higher scores.

Overall, the UGF approach provides an explicit and concise understanding of urban geo-climatic conditions, also integrating natural hazards, climatic pressures, and human impacts. It highlights local differences often masked by traditional indicators and offers a valuable tool for evidence-based urban planning, climate adaptation, risk reduction, and sustainable urban regeneration. The methodology emphasizes the recognition of the subsurface as a primary urban infrastructure, essential for resilient city development.

 

Lentini, A., Galve, J. P., Benjumea, B., Bricker, S., Devleeschouwer, X., Guarino, P. M., Kearsey, T., Leoni, G., Puzzilli, L. M., Romeo, S., Venvik, G., & La Vigna, F. (2024). The Urban Geo-climate Footprint approach: Enhancing urban resilience through improved geological conceptualisation. Cities, 145, 105287. https://doi.org/10.1016/j.cities.2024.105287 

How to cite: Romeo, S., Bonasera, M., Campolunghi, M. P., Di Paola, G., Guarino, P. M., Leoni, G., Proietti, R., and La Vigna, F.: Urban Geo-climate Footprint (UGF) for Classifying Italian Cities by Geological and Climatic Features, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18030, https://doi.org/10.5194/egusphere-egu26-18030, 2026.

Coastal port-city regions operate as intricate urban systems, where transport infrastructure, land-use change, environmental limits, and socio-economic forces interact across multiple spatial and temporal scales. In rapidly evolving coastal cities, port-led development may bring economic opportunities, but it also tends to introduce new environmental risks and social tensions. This duality is especially visible in cities where growth is unfolding faster than planning frameworks can adapt, which suggests a need for analytical approaches that are both integrated and spatially grounded. This study develops a multi-criteria spatial framework to assess land suitability and identify potential growth nodes along the Vizhinjam-Trivandrum corridor in southern India shaped by the development of the Vizhinjam International Seaport.

The framework integrates multi-temporal remote sensing data, geospatial indicators, and expert-derived weights using the Analytic Hierarchy Process (AHP) within a GIS environment. Land-use and land-cover dynamics from 2005 to 2025 are analysed alongside transport connectivity, environmental sensitivity, geo-hazard exposure, economic feasibility, and socio-regulatory constraints. These factors are represented as interconnected components of the urban system. To balance analytical rigour with practical applicability, literature-based indicators are consolidated into a concise hierarchical structure. This structure encompasses physical environmental, infrastructural, economic, and socio-community dimensions. Expert judgement is incorporated through structured pairwise comparisons, producing a transparent and reproducible weighting scheme.

The resulting analysis produces a spatial suitability surface that highlights development potential and constraints across the corridor. Early findings indicate that proximity to port infrastructure and transport connectivity strongly influence emerging growth patterns. At the same time, this advantage is often offset by environmental sensitivity and hazard exposure. These overlaps point to some of the core trade-offs that define port-city development, particularly in ecologically fragile coastal settings. By combining urban change monitoring with spatial decision-support analysis, the proposed framework demonstrates the value of integrated approaches for supporting sustainable and resilient development in complex coastal urban environments.

How to cite: Bala, D., Paul, S. K., and Yadav, A.: A Multi-Criteria Spatial Modelling Framework for Port-Urban Growth in a Coastal City System: The Vizhinjam-Trivandrum Corridor, India , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18190, https://doi.org/10.5194/egusphere-egu26-18190, 2026.

EGU26-18358 | ECS | Orals | ITS3.12/NP8.8

Fine-scale covariation of residential heating emissions and socioeconomic variables across Germany: implications for urban climate policy 

Sebastian Block, Veit Ulrich, Gefei Kong, Maria Martin, and Kirsten von Elverfeldt

Residential heating is a large source of greenhouse gas emissions and a priority for urban climate change mitigation efforts. However, effective planning of decarbonization policies is hampered by the lack of fine-resolution emission estimates at sub-city scales. Such spatially disaggregated data are essential for analyzing how emission patterns co-vary with important social, economic, and demographic characteristics within cities, which is needed for designing targeted and equitable policy interventions.

We use high-resolution population and building data from the 2022 German census to estimate carbon dioxide emissions from residential buildings across Germany. We then explore how emission patterns covary with socioeconomic and demographic variables relevant for policy design.

Our analysis reveals significant spatial heterogeneity in per capita emissions within cities. We find that areas with higher rates of home ownership exhibit elevated per capita emissions, suggesting these neighborhoods represent prime targets for building renovation incentives directed at homeowners. Additionally, we observe higher per capita emissions in areas with larger proportions of senior residents (>66 years old), who typically consume more energy for heating. This pattern indicates that high-emitting buildings (larger, older buildings heated with carbon-intensive energy carriers) tend to spatially overlap with populations likely to have intensive heating behaviors, potentially compounding resulting emissions.

These findings underscore the importance of analyzing urban carbon dioxide emission patterns at fine spatial scales and examining their spatial correlation with relevant socioeconomic and demographic characteristics. Our analysis reveals sub-city emission patterns with clear implications for policy design. Effective decarbonization strategies must account for these spatial patterns to plan interventions that account both for building infrastructure and occupant characteristics, ensuring efficient resource allocation and equitable climate action across diverse urban settings.

 

How to cite: Block, S., Ulrich, V., Kong, G., Martin, M., and von Elverfeldt, K.: Fine-scale covariation of residential heating emissions and socioeconomic variables across Germany: implications for urban climate policy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18358, https://doi.org/10.5194/egusphere-egu26-18358, 2026.

EGU26-19378 | ECS | Posters on site | ITS3.12/NP8.8

Urban scaling of well-being, a cross-country comparison 

Mirjam van Hemmen, Arend Ligtenberg, Sytze de Bruin, Clive Sabel, Gerrit Gort, Corne Vreugdenhil, Hannah Frome, Dan Foy, and Kirsten Maria de Beurs

Cities are complex systems and its many components strongly interrelated. Still, urban scaling studies have observed regularities in urban output across multiple national urban systems. Urban scaling studies examine how urban characteristics change systematically with population size. Previous research has shown that socio-economic outputs, such as GDP and patents, typically scale superlinearly, meaning that they increase more than proportionally with population size. In contrast, infrastructural quantities, such as road length, tend to scale sublinearly. Beyond average trends, scaling residuals identify cities that over- or underperform relative to their size, offering insights into additional drivers of urban outcomes and a tool for monitoring policy impacts.

 

While urban scaling research has largely focused on socio-economic and infrastructural features, studies have shown that health indicators such as obesity, smoking, diabetes and influenza also exhibit scaling relationships with city size. Moreover, recent work has found non-linear scaling relationships for well-being indicators in Dutch cities. However, urban well-being scaling has not yet been examined systematically across different national contexts. It therefore remains unknown whether the observed relationships between city size and well-being are the same across different national contexts. Furthermore, the potential of scaling residuals analysis for well-being policy remains to be explored.

 

This study uses a unique dataset provided by Gallup to study urban scaling for well-being for 18 countries, with varying geographical contexts and economic development stages. The dataset covers a range of topics related to well-being. The same questions and methodology are used for all countries, enabling country comparisons. We show that some well-being indicators exhibit scaling relationships and that scaling relationships depend on the country context. In addition, we explore whether out- or underperforming cities share common urban environmental characteristics.

With current rapid urbanisation it is important to increase our understanding of urban – well-being interactions. Urban scaling studies of well-being can increase our understanding of well-being patterns and outliers in a system of cities.

How to cite: van Hemmen, M., Ligtenberg, A., de Bruin, S., Sabel, C., Gort, G., Vreugdenhil, C., Frome, H., Foy, D., and de Beurs, K. M.: Urban scaling of well-being, a cross-country comparison, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19378, https://doi.org/10.5194/egusphere-egu26-19378, 2026.

EGU26-19442 | ECS | Posters on site | ITS3.12/NP8.8

Estimating urban albedo and emissivity from street view imagery 

Peter Kalverla, Bart Schilperoort, Alexander Hadjiivanov, Gert-Jan Steeneveld, Wim Timmermans, Bianca Eline Sandvik, Dragan Milosevic, Srinidhi Gadde, and Victoria Hafkamp

Weather and climate simulations continue to evolve towards higher resolutions. This allows them to resolve small-scale processes more explicitly, but the added value is constrained by the availability of accurate localized data, particularly in urban areas where there is a large variety in urban structures and surface properties. Currently, mesoscale models like WRF rely on typological classifications such as the Local Climate Zones. Despite their proven effectiveness, they bundle multiple properties into a single urban class, which means individual parameters cannot be represented independently. Recent studies have introduced fine-scale explicit datasets on various urban properties such as building heights and vegetation fraction. But to the best of our knowledge, local datasets of albedo and emissivity of urban surfaces are not available at scale. 

In the “Urban-M4” project, we are exploring whether street view imagery can provide these missing radiative properties for use in urban weather models. Such imagery is widely available nowadays, either as proprietary data (e.g. Google Streetview), but also increasingly as open data from municipalities or through crowdsourcing platforms such as Mapillary and Kartaview. Simultaneously, computer vision methods have become much more powerful. State of the art models can now perform advanced tasks including detection of a wide range of objects and materials based on free prompts. This allows us to extract individual buildings or building parts from street view images and analyse their characteristics. As a proxy for albedo, we have been experimenting with various brightness metrics of building pixels, resulting in a first preliminary map of façade albedo for Amsterdam based on 100k images. We are currently setting up an observational campaign to validate and refine this method. To eventually estimate emissivity as well, we are investigating the capability of existing computer vision models to recognize (urban) materials. 

We are developing this openly on GitHub, and to facilitate adoption the functionality is bundled in a Python package called ‘streetscapes’. It includes tools for retrieving images from various sources and running a number of computer vision models. While it is possible to automatically segments millions of images, the quality of the results is still affected by the heterogeneity of images and the varying accuracy of the models. Therefore, we aim to further develop the package to accommodate a ‘human-in-the-loop’ workflow, so it becomes manageable to inspect images and their metadata in a spatial context, and filter or modify images and metadata from a graphical interface. We have modified WRF to enable ingestion of 2D maps of urban albedo and emissivity and are preparing the first tests.

How to cite: Kalverla, P., Schilperoort, B., Hadjiivanov, A., Steeneveld, G.-J., Timmermans, W., Sandvik, B. E., Milosevic, D., Gadde, S., and Hafkamp, V.: Estimating urban albedo and emissivity from street view imagery, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19442, https://doi.org/10.5194/egusphere-egu26-19442, 2026.

EGU26-19640 | ECS | Orals | ITS3.12/NP8.8

Bridging Scales and Processes: A Land Surface Model Framework for the Urban Thermal Environment 

Lingbo Xue, Quang-Van Doan, Hiroyuki Kusaka, Cenlin He, and Fei Chen

More than half of the world’s population currently lives in cities, and the urban population is expected to reach two-thirds of the total population by 2050. As the IPCC report pointed out, the growing urban population faces heightened climate-related risks, including sea-level rise, thermal stress, tropical cyclones, heavy rainfall, etc. Of these, extreme heat stands out as one of the most important and serious urban meteorological hazards. A well-documented example is the urban heat island (UHI), which could be amplified by heatwaves (HW). However, investigating these complex interactions is often hindered by the lack of high-quality, high-resolution climate information. While regional climate models are commonly used to downscale GCMs, their heavy computational demands limit their applicability for multi-scenario urban studies. In this study, we proposed a new approach using offline land surface models to downscale reanalysis data and acquire 2m air temperature and surface temperature. Using HRLDAS/Noah-MP as an example, this accounts for diverse sub-components—such as vegetation, impervious surfaces, and anthropogenic heat—through a sub-grid tiling scheme. By explicitly simulating the energy and water exchanges within urban and natural tiles, our approach effectively captures the fine-grained thermal heterogeneity of the city. To further enhance the physical representation of urban energy and water cycles, we integrated multiple land surface models, such as SUWES and MATSIRO, into the framework. This approach provides a robust, low-cost tool for predicting near-surface thermal conditions, offering valuable insights for urban planning and the enhancement of citizen well-being in the face of a warming climate.

How to cite: Xue, L., Doan, Q.-V., Kusaka, H., He, C., and Chen, F.: Bridging Scales and Processes: A Land Surface Model Framework for the Urban Thermal Environment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19640, https://doi.org/10.5194/egusphere-egu26-19640, 2026.

Large language models (LLMs) offer the potential to make complex scientific software accessible through natural language interfaces. However, LLMs hallucinate by design—generating plausible but incorrect physics, inventing parameter values, and confidently explaining non-existent model features. For scientific computing, this poses unacceptable risks to research integrity.

We present a solution: a Model Context Protocol (MCP) server for the Surface Urban Energy and Water balance Scheme (SUEWS). MCP, introduced by Anthropic in 2024 and now adopted by major AI providers, enables a fundamental architectural shift from AI-generated code to AI-orchestrated validated operations. Rather than prompting an LLM to write Python code and hoping it implements correct physics, we provide 15 typed tools with validated inputs and outputs. The AI can orchestrate these tools but cannot bypass validation or invent new operations.

The SUEWS-MCP server implements tools across five categories: configuration (create, update, validate, inspect), knowledge (list models, access schema, retrieve physics implementations), simulation (run SUEWS), utilities (calibrate OHM coefficients, document variables), and analysis (load and export results). Each tool enforces physical constraints—albedo must lie between 0 and 1, temperatures must exceed 0 K—rejecting invalid configurations before computation.

A key innovation addresses hallucination at the knowledge level. When explaining how SUEWS calculates storage heat flux, the AI retrieves and interprets actual Fortran source code rather than generating explanations from training data. If the implementation changes, the explanation changes. This direct coupling between AI responses and model code ensures trustworthy scientific communication.

We evaluated the system using 50 test questions across difficulty levels, comparing four configurations: baseline (no tools), reference (full repository access), and two MCP-enabled models. MCP improved answer accuracy by 18–20% over baseline, with largest gains on physics questions requiring equations and implementation details. The smaller model with MCP tools outperformed the larger model, demonstrating that tool access matters more than model size for domain-specific applications.

This work demonstrates that AI can make scientific software accessible without sacrificing rigour. Natural language interfaces become viable for urban climate modelling when AI orchestrates validated operations rather than generating unchecked code. The approach generalises: any computational tool with well-defined operations can expose an MCP interface, enabling trustworthy AI assistance across scientific domains.

How to cite: Sun, T.: Talking to Cities: A Model Context Protocol Server for SUEWS, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20672, https://doi.org/10.5194/egusphere-egu26-20672, 2026.

EGU26-21394 | ECS | Posters on site | ITS3.12/NP8.8

From single buildings to cities: accurate LOD modelling from tiled airborne cross-source point clouds. 

Shahoriar Parvaz and Felicia Norma Teferle

City-scale 3D building modelling is essential for understanding complex cities, but it remains difficult due to heterogeneous data sources. The process is particularly challenging with cross-sourced point clouds and processing them in tiles. Differences in density and noise between LiDAR and photogrammetry, combined with tile boundaries that cut through buildings, often lead to incomplete or inconsistent models.
In this study, we extend the plane-based reconstruction method originally designed for single buildings to work at a city scale. We propose a workflow that handles tiles intelligently. By using buffered processing and clustering, we ensure that buildings spanning multiple tiles are reconstructed completely. We also introduce a strategy to assign each building to a single tile, which avoids duplicates and keeps the process scalable. We evaluated this approach in dense urban areas with diverse building types. The results show that the method generates consistent models across tile boundaries while maintaining high geometric accuracy. This framework supports automated modelling of large areas and provides a solid foundation for analyzing complex built environments.

How to cite: Parvaz, S. and Teferle, F. N.: From single buildings to cities: accurate LOD modelling from tiled airborne cross-source point clouds., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21394, https://doi.org/10.5194/egusphere-egu26-21394, 2026.

EGU26-1228 | ECS | Orals | ITS4.1/NP8.9

An early warning indicator for tipping in a strongly forced system 

Isobel Parry, Paul Ritchie, and Peter Cox

Classical critical slowing down early warning signals (observing increasing trends in the autocorrelation and variance) have been developed to try and detect when a system is approaching a tipping point, typically represented mathematically by a bifurcation.  However, these signals often fail for strongly forced slow systems. Here we propose a new method that reconstructs the quasi-equilibrium state and therefore produces a robust indication of where the critical threshold may lie in a system.

We show that the variance of this reconstructed quasi-equilibrium state increases exponentially ahead of its critical threshold, at time tcrit, for both strongly forced fast and slow systems. Using both the reconstructed quasi-equilibrium state and the inverse of its variance allows us to diagnose the location of the critical threshold for a strongly forced, slow system which has passed the critical threshold but not yet tipped, and where classical critical slowing down indicators often fail. 

How to cite: Parry, I., Ritchie, P., and Cox, P.: An early warning indicator for tipping in a strongly forced system, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1228, https://doi.org/10.5194/egusphere-egu26-1228, 2026.

The intrinsic variability of the Gulf Stream (GS), the abrupt transition that can occur at a certain tipping point and the early warning signals that precede it, are investigated through a process modeling study. The nonlinear reduced-gravity shallow water equations are solved with schematic but quite realistic geometric configuration and time-independent wind forcing. A reference simulation shows a GS with correct mean Florida Current (FC) transport, realistic separation at Cape Hatteras (CH) due to inertial overshooting, realistic northern recirculation gyre and a strong chaotic intrinsic variability.

To simulate the effect of anthropogenic forcing, a sensitivity analysis is performed by decreasing the forcing amplitude. The results show a gradual shift of the GS toward the coasts north of CH and, therefore, a connection between the decline of the FC and one of the most significant fingerprints of a weakened Atlantic Meridional Overturning Circulation (AMOC). Furthermore, at a tipping point there is an abrupt transition to a GS flowing along the coasts north of CH; this is preceded by an early warning characterized by the fluctuation-dissipation relation, which is revealed by an increase in the autocorrelation and variance of the signals. It is suggested that such critical behavior could impact the AMOC tipping element. As regards the intrinsic variability of the Mediterranean Sea circulation, preliminary results are presented based on ensemble simulations using the FESOM-C finite element model. This research was partially supported by the INVMED project funded by the Italian PRIN-2022.

How to cite: Pierini, S.: Intrinsic oceanic variability, tipping points and early warning signals: examples from the dynamics of the Gulf Stream and the Mediterranean Sea , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2849, https://doi.org/10.5194/egusphere-egu26-2849, 2026.

EGU26-3250 | ECS | Posters on site | ITS4.1/NP8.9

Warming-driven rise in soil moisture entropy signals destabilization of the Asian Water Tower 

Yiran Xie, Teng Liu, Xuan Ma, Yingshuo Lyu, Xu Wang, Yatong Qian, Yongwen Zhang, Ming Wang, and Xiaosong Chen

The Tibetan Plateau (TP), known as the "Asian Water Tower," is currently undergoing a rapid wetting trend. While this moisture increase is commonly viewed as beneficial for water availability, it remains unclear whether the hydrological system itself is becoming more resilient, and whether continued warming could push it toward instability. Here, we apply an entropy-based framework to quantify the changing structural organization of the TP's soil moisture system. We show that from 2000 to 2024, regional wetting has driven a long-term decline in entropy, reflecting an increase in system order and stability due to enhanced hydrological buffering capacity. This stability is modulated by the El Niño-Southern Oscillation (ENSO), which regulates regional heterogeneity via a distinct spatial dipole. Crucially, however, CMIP6 climate projections reveal an alarming reversal: entropy increases under continued warming and regional contrasts intensify, with some models exhibiting an abrupt mid-century transition. Our findings suggest that while current wetting provides a stabilizing buffer, continued warming is projected to amplify spatial heterogeneity, thereby destabilizing the Asian Water Tower, with significant risks for downstream water security.

How to cite: Xie, Y., Liu, T., Ma, X., Lyu, Y., Wang, X., Qian, Y., Zhang, Y., Wang, M., and Chen, X.: Warming-driven rise in soil moisture entropy signals destabilization of the Asian Water Tower, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3250, https://doi.org/10.5194/egusphere-egu26-3250, 2026.

EGU26-3854 | Orals | ITS4.1/NP8.9

Predicting Instabilities in Transient Landforms and Interconnected Ecosystems 

Taylor Smith, Andreas Morr, Bodo Bookhagen, and Niklas Boers

Many parts of the Earth system are thought to have multiple stable equilibrium states, with the potential for catastrophic shifts between them. Common methods to assess system stability require stationary (trend- and seasonality-free) data, necessitating error-prone data pre-processing. Here, we use Floquet Multipliers to quantify the stability of periodically-forced systems of known periodicity (e.g., annual seasonality) using diverse data without pre-processing. We demonstrate our approach using synthetic time series and spatio-temporal vegetation models, and further investigate two real-world systems: mountain glaciers and the Amazon rainforest. We find that glacier surge onset can be predicted from surface velocity data and that we can recover spatially explicit destabilization patterns in the Amazon. Our method is robust to changing noise levels, such as those caused by merging data from different sensors, and can be applied to quantify the stability of a wide range of spatio-temporal systems, including climate subsystems, ecosystems, and transient landforms.

How to cite: Smith, T., Morr, A., Bookhagen, B., and Boers, N.: Predicting Instabilities in Transient Landforms and Interconnected Ecosystems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3854, https://doi.org/10.5194/egusphere-egu26-3854, 2026.

EGU26-3945 | ECS | Posters on site | ITS4.1/NP8.9

The influence of data gaps and outliers on resilience indicators 

Teng Liu, Andreas Morr, Sebastian Bathiany, Lana L. Blaschke, Zhen Qian, Chan Diao, Taylor Smith, and Niklas Boers

The resilience, or stability, of major Earth system components is increasingly threatened by anthropogenic pressures, demanding reliable early warning signals for abrupt and irreversible regime shifts. Widely used data-driven resilience indicators based on variance and autocorrelation detect 'critical slowing down', a signature of decreasing stability. However, the interpretation of these indicators is hampered by poorly understood interdependencies and their susceptibility to common data issues such as missing values and outliers. Here, we establish a rigorous mathematical analysis of the statistical dependency between variance- and autocorrelation-based resilience indicators, revealing that their agreement is fundamentally driven by the time series' initial data point. Using synthetic and empirical data, we demonstrate that missing values substantially weaken indicator agreement, while outliers introduce systematic biases that lead to overestimation of resilience based on temporal autocorrelation. Our results provide a necessary and rigorous foundation for preprocessing strategies and accuracy assessments across the growing number of disciplines that use real-world data to infer changes in system resilience.

How to cite: Liu, T., Morr, A., Bathiany, S., Blaschke, L. L., Qian, Z., Diao, C., Smith, T., and Boers, N.: The influence of data gaps and outliers on resilience indicators, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3945, https://doi.org/10.5194/egusphere-egu26-3945, 2026.

EGU26-4250 | ECS | Orals | ITS4.1/NP8.9

Critical freshwater forcing for AMOC tipping in climate models – compensation matters 

Oliver Mehling, Elian Vanderborght, and Henk A. Dijkstra

Ocean and climate models of various complexity have shown that the Atlantic Meridional Overturning Circulation (AMOC) can undergo tipping as a function of freshwater forcing. Most of these model experiments compensate for the freshwater input to conserve global salinity, with salt being added either at the surface or throughout the ocean volume. However, these two different compensation methods have so far only been compared in a single, coarse-resolution climate model, and therefore little is known robustly about the effect of salinity compensation on the AMOC tipping point. Here, using an ocean model at 1° resolution and an intermediate-complexity coupled climate model, we systematically compare the effect of surface vs volume compensation on the tipping point of the AMOC as diagnosed from quasi-equilibrium experiments using a freshwater flux over the region 20°N–50°N.

Salinity compensation at the surface consistently delays AMOC tipping compared to volume compensation. This is mainly because the compensation salinity added over the subpolar North Atlantic counteracts the weakening salinity gradient from freshwater forcing. In contrast, the compensation method does not strongly impact AMOC recovery when tracing the full hysteresis loop. Our results indicate that the distance of present-day climate to the AMOC tipping point with respect to freshwater forcing might have been overestimated in recent modeling studies, compounding the effect of model biases.

How to cite: Mehling, O., Vanderborght, E., and Dijkstra, H. A.: Critical freshwater forcing for AMOC tipping in climate models – compensation matters, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4250, https://doi.org/10.5194/egusphere-egu26-4250, 2026.

EGU26-4350 | ECS | Orals | ITS4.1/NP8.9

Phase Transition in the Atlantic Surface Currents 

Han Huang, Ningning Tao, Hongyu Wang, Teng Liu, Fei Xie, Xichen Li, Yongwen Zhang, Niklas Boers, Jingfang Fan, Deliang Chen, and Xiaosong Chen

The Atlantic surface ocean currents, connecting the atmosphere and the deep ocean currents like the Atlantic Meridional Overturning Circulation (AMOC), plays a central role in regulating Earth’s climate. Yet how large-scale surface currents respond to ongoing climate change remains poorly constrained. Here we identify a previously unrecognized phase of Atlantic surface circulation, termed the Atlantic Convergence–Divergence Mode (ACDM), characterized by a convergence–divergence structure in the North Atlantic and coherent meridional flows in the South Atlantic. We find that the ACDM has experienced a transition evidenced by a systematic weakening of vertical water exchange and meridional flows, with its interannual variability marking a regime shift in 2009, consistent with the RAPID-MOCHA AMOC observations. Our analysis indicates that this shift is driven by AMOC-modulated ocean-atmosphere interactions, including the North Atlantic Oscillation (NAO) and layered ocean heat transport.  We therefore propose the ACDM’s interannual variability as a more sensitive proxy for AMOC at interannual timescales, revealing the coexistence of a gradual multidecadal decrease trend and an abrupt interannual shift in AMOC variability. Moreover, this step-like shift in AMOC also suggests the important role of atmospheric disturbances and reveal that AMOC may be more delicate and closer to tipping point than  than previously anticipated. These findings confirm that AMOC variability can trigger rapid, large-scale transitions in surface circulation, pushing it into a new, weaker phase.

How to cite: Huang, H., Tao, N., Wang, H., Liu, T., Xie, F., Li, X., Zhang, Y., Boers, N., Fan, J., Chen, D., and Chen, X.: Phase Transition in the Atlantic Surface Currents, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4350, https://doi.org/10.5194/egusphere-egu26-4350, 2026.

EGU26-4473 | ECS | Orals | ITS4.1/NP8.9

Deterministic Collapse and Stochastic Recovery in a Data-Driven Model of the Atlantic Meridional Overturning Circulation 

Qi-fan Wu, Dion Häfner, Roman Nuterman, Guido Vettoretti, and Markus Jochum

During the last ice-age, temperatures in Greenland have frequently increased and decreased by 10°C. Detailed studies with climate models suggest that this is caused by collapses and recoveries of the Atlantic Meridional Overturning Circulation (AMOC). The causes of these AMOC transitions are still debated, though. Here we describe the development of a neural-network based surrogate model of the AMOC. It is trained on 32,000 years of climate model integrations to build a set of stochastic differential equations that emulate the climate models' AMOC behavior. In particular it reproduces the spectra and the asymmetry in the times it takes for the AMOC to recover and collapse, which makes it more realistic than previously published sets of coupled differential equations to study past AMOC transitions. Monte Carlo simulations with this model show that collapses are deterministic, but recoveries are stochastically forced, in partial support of the leading hypotheses surrounding the AMOC transitions. 

How to cite: Wu, Q., Häfner, D., Nuterman, R., Vettoretti, G., and Jochum, M.: Deterministic Collapse and Stochastic Recovery in a Data-Driven Model of the Atlantic Meridional Overturning Circulation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4473, https://doi.org/10.5194/egusphere-egu26-4473, 2026.

EGU26-4490 | ECS | Orals | ITS4.1/NP8.9

Pinpointing Amazon forest tipping in global warming and deforestation pathways 

Nico Wunderling, Boris Sakschewski, Johan Rockström, Bernardo M. Flores, Marina Hirota, and Arie Staal

Humanity is exerting unprecedented pressure on the Amazon forest through global warming, deforestation, land-use change, and large-scale infrastructure projects. As the Amazon may exhibit a tipping point beyond which detrimental changes become self-propelling, these pressures could trigger system-wide state shifts. We use a dynamical systems model to assess local transition risks and cascading transitions across the Amazon under different SSP-scenarios (SSP2-4.5, SSP3-7.0 and SSP5-8.5). For each scenario, atmospheric moisture transport is derived throughout the 21st century using an established moisture-tracking model.

In the absence of deforestation, we identify a critical global warming threshold of 3.7-4.0 °C, beyond which around one third of the Amazon loses stability. When deforestation is included, however, our simulations indicate a near system-wide transition (62-77% of the forest area) at global warming levels of 1.5-2.0°C combined with 20-30% deforestation across the basin. Most transitions are driven by drought-induced knock-on effects, causing long-range cascading impacts through the lack of atmospheric moisture recycling. Overall, our results highlight the need to limit warming to as close to 1.5 °C as possible and, halt deforestation at current levels (~17% across the basin), while ideally restoring degraded areas to reduce transition risks across the Amazon forest.

How to cite: Wunderling, N., Sakschewski, B., Rockström, J., Flores, B. M., Hirota, M., and Staal, A.: Pinpointing Amazon forest tipping in global warming and deforestation pathways, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4490, https://doi.org/10.5194/egusphere-egu26-4490, 2026.

Escalating climate crises, characterized by rising sea levels, alongside excessive groundwater pumping, have severely exacerbated saltwater intrusion, posing a critical threat to coastal aquifers. These combined environmental stressors induce complex, non-linear dynamics in groundwater systems, making the exact prediction of regime shifts driven by tipping points increasingly challenging. To address these uncertainties, this study proposes a comprehensive data-driven approach designed to identify early warning signals (EWS) for approaching tipping points using Electrical Conductivity (EC) time-series data. The primary objective is to investigate the feasibility of utilizing complementary statistical indicators—Variance and Fisher Information (FI)—to assess system instability. We analyzed monitoring data from Incheon and Jeju, South Korea, to validate whether these metrics can effectively filter noise and detect genuine precursor signals. Empirical results demonstrate that our approach achieves significantly enhanced performance in distinguishing critical transitions compared to single-indicator methods. Ultimately, this study serves as a foundational step towards establishing an "Integrated Machine Learning" framework. By validating these statistical metrics as key features, we aim to incorporate them into advanced learning algorithms to further improve the robustness and predictive accuracy of coastal groundwater management systems against climate-induced risks.

Acknowledgement
This work was supported by National Research Foundation of Korea(NRF) grant funded by the Ministry of Science and Technology (RS-2024-00356786).

How to cite: Heo, E., Kim, S., and Park, J.: A Comprehensive Data-Driven Approach for Detecting Regime Shifts in Coastal Groundwater: Towards an Integrated Machine Learning Framework, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4647, https://doi.org/10.5194/egusphere-egu26-4647, 2026.

EGU26-4958 | Orals | ITS4.1/NP8.9

Permafrost as a tipping element in the Earth System: scales matter 

Victor Brovkin, Thomas Kleinen, Philipp de Vrese, and Annett Bartsch

The permafrost soils in the northern high latitudes contain about twice as much carbon as the atmosphere. This organic soil matter has accumulated over many thousands of years and is now exposed to anthropogenic warming, which is amplified by a factor of three to four in the Arctic compared to global warming.  The thawed organic matter is mineralized and released into the atmosphere as CO2 or CH4, which amplifies ongoing warming (permafrost carbon feedback). In addition, the thawing of permafrost soils leads to changes in land surface hydrology and potential drainage, which could also amplify global warming due to the decrease in summer cloud cover (permafrost cloud feedback). The permafrost changes impact other regions and Earth tipping elements, including tropical forests.

Are permafrost feedbacks nonlinear, is there a threshold for global warming above which the feedbacks lead to disproportional increase in carbon thaw? Future projections using Earth system and land surface models suggest a rather linear permafrost response to global warming, but they are mostly based on gradual thawing processes and do not take into account abrupt thawing and extreme events. Numerous processes that lead to abrupt thawing at the local level, such as thermokarst, lake formation and drainage, or surface subsidence, have been neglected in large-scale models to date. We will present the results of model experiments and discuss the potential impact of these missing processes on the nonlinear response, as well as indicators of multistability of carbon and hydrology at different scales. We will also discuss irreversibility of permafrost changes and their response timescales as supported by paleo evidence. 

How to cite: Brovkin, V., Kleinen, T., de Vrese, P., and Bartsch, A.: Permafrost as a tipping element in the Earth System: scales matter, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4958, https://doi.org/10.5194/egusphere-egu26-4958, 2026.

EGU26-5042 | ECS | Orals | ITS4.1/NP8.9

Resilience Loss of Tropical Forests in Recent Decades 

Lana Blaschke, Sebastian Bathiany, Marina Hirota, and Niklas Boers

In view of ongoing climate and land use change, the resilience of tropical forests is crucial for maintaining ecosystem services and  preventing potential forest loss and associated greenhouse gas emissions. Recent studies have attempted to quantify tropical forest resilience changes using different satellite vegetation products. However, it has not been assessed to what extent the data satisfies the theoretical assumptions of the employed resilience metrics. Here, we propose a framework to determine the most reliable combination of vegetation data and metrics to monitor resilience from space. We apply our framework to select the best combinations from 16 vegetation products and nine resilience metrics.  Based on these, we consistently find that tropical forests in South America, Africa, and Asia have experienced a decline in resilience over recent decades. Our robust assessment of resilience changes in tropical forests has important implications for targeted actions to prevent further tropical forest loss.

How to cite: Blaschke, L., Bathiany, S., Hirota, M., and Boers, N.: Resilience Loss of Tropical Forests in Recent Decades, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5042, https://doi.org/10.5194/egusphere-egu26-5042, 2026.

EGU26-6440 | ECS | Posters on site | ITS4.1/NP8.9

Meltwater from West Antarctic Ice Sheet Tipping Impacts AMOC Resilience 

Sacha Sinet, Anna S von der Heydt, and Henk A Dijkstra

The Atlantic Meridional Overturning Circulation (AMOC) and polar ice sheets are coupled tipping elements of the Earth system, allowing for potential cascading tipping events in which tipping is facilitated by their mutual interactions. However, while an AMOC destabilization driven by Greenland Ice Sheet (GIS) meltwater release is well-documented, the consequences of a West Antarctic Ice Sheet (WAIS) tipping on the AMOC remain unclear. In the Earth system Model of Intermediate Complexity CLIMBER-X, we perform experiments where meltwater fluxes representing plausible tipping trajectories of the GIS and WAIS are applied. We find that WAIS meltwater input can increase or decrease the AMOC resilience to GIS meltwater. In particular, for the first time in a comprehensive model, we show that WAIS meltwater can prevent an AMOC collapse. Moreover, we find this stabilzation to occur for ice sheet tipping trajectories that are relevant under high future greenhouse gas emission scenarios.

How to cite: Sinet, S., von der Heydt, A. S., and Dijkstra, H. A.: Meltwater from West Antarctic Ice Sheet Tipping Impacts AMOC Resilience, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6440, https://doi.org/10.5194/egusphere-egu26-6440, 2026.

EGU26-6567 | ECS | Orals | ITS4.1/NP8.9

Emulating tipping elements: Linking Earth system models to low-order dynamics for tipping elements 

Nils Bochow, Jonathan Krönke, Julius Garbe, and Nico Wunderling

Crossing climate tipping points poses a rising risk under continued global warming. 
Yet quantitative tipping risk assessments often rely on idealised system dynamics and do not take into account Earth system model (ESM) processes. 
Here, we present a process-informed, updatable framework that links systematic stability assessments from comprehensive models to transparent low-order dynamical systems for three high-impact climate tipping elements (TEs): the Atlantic Meridional Overturning Circulation (AMOC), the Greenland Ice Sheet (GrIS), and the West Antarctic Ice Sheet (WAIS). 
We assemble TE experiments from Earth system and Earth system component models, fit element-specific dynamical systems with saddle-node bifurcations that map external forcing to state transitions, and run idealised instantaneous-forcing experiments to show the application of our framework.
A simple, modular update protocol allows tipping thresholds and timescales to be revised as new simulations from ESMs become available without refitting the full framework. 
Applied to current ESM simulations, our emulators reproduce multistability of the GrIS and WAIS and a freshwater-forced weakening of the AMOC, yielding decision-relevant transient and equilibrium behaviour consistent with the underlying ESMs. 
Our approach provides a transparent bridge between comprehensive simulations and risk metrics, and can be extended to additional climate tipping elements as suitable experiments become available.

How to cite: Bochow, N., Krönke, J., Garbe, J., and Wunderling, N.: Emulating tipping elements: Linking Earth system models to low-order dynamics for tipping elements, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6567, https://doi.org/10.5194/egusphere-egu26-6567, 2026.

EGU26-7606 | ECS | Posters on site | ITS4.1/NP8.9

The Interdecadal Bipolar Oscillation: A Potential Driver for Rapid Antarctic Climate Transitions 

Hongyu Wang, Jingfang Fan, Fei Xie, Jingyuan Li, Rui Shi, Yan Xia, Deliang Chen, and Xiaosong Chen

The polar regions are critical components of complex Earth systems, housing potential tipping elements such as the West Antarctic Ice Sheet and sea ice systems. However, the climate trajectories of the two poles have diverged significantly over the past century. While the Arctic has exhibited rapid warming and dramatic sea ice loss—a phenomenon known as Arctic amplification—the Antarctic has shown a delayed and more heterogeneous response. Observations indicate that prior to the late 1980s, parts of Antarctica experienced warming and moistening while the Arctic remained relatively stable; subsequently, this pattern reversed, with the Arctic undergoing accelerated change while the Antarctic trend slowed or displayed spatial variability. Understanding the drivers of polar climate variability is paramount for anticipating potential abrupt transitions or tipping points in the regions.

Here, we identify a robust internal variability mode in atmospheric water vapor—termed the Interdecadal Bipolar Oscillation (IBO)—that provides a physical explanation for these historical asymmetries. Using the eigen microstate theory on ERA5 reanalysis and CMIP6 simulations (historical, piControl, and SSPs), we reveal that the IBO links the Arctic and Antarctic in a quasi-periodic (60–80 years) seesaw pattern. We demonstrate that the IBO has modulated interdecadal asymmetries in polar climate change over the past 80 years. Specifically, a phase shift in the late 1980s accelerated Arctic moistening while suppressing similar changes in the Antarctic.

Crucially, our projections under various Shared Socioeconomic Pathways (SSPs) indicate an imminent IBO phase reversal in the coming decades. This transition is expected to shift the IBO from a dampening to an amplifying phase for the Antarctic, coinciding with the background global warming signal. We suggest that this alignment could trigger a regime shift toward rapid Antarctic moistening and warming, potentially destabilizing the ice sheet–atmosphere interactions. The IBO thus acts as a critical internal regulator that may modulate the distance to tipping points in the polar climate system. By elucidating the interplay between this internal oscillation and external anthropogenic forcing, our study offers new insights into the mechanisms that could precipitate abrupt climate transitions in the Antarctic.

How to cite: Wang, H., Fan, J., Xie, F., Li, J., Shi, R., Xia, Y., Chen, D., and Chen, X.: The Interdecadal Bipolar Oscillation: A Potential Driver for Rapid Antarctic Climate Transitions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7606, https://doi.org/10.5194/egusphere-egu26-7606, 2026.

EGU26-8429 | ECS | Orals | ITS4.1/NP8.9

The interaction between the Amazon rainforest and the AMOC 

Chiara Stanchieri, Henk A. Dijkstra, Robbin Bastiaansen, Kobe De Maeyer, Max Rietkerk, and Arie Staal

The Atlantic Meridional Overturning Circulation (AMOC) is a major component of the global ocean circulation and plays a crucial role in regulating Earth’s climate. Similarly, the Amazon Rainforest (ARF), often referred to as the “lungs of the planet”, is a key regulator of the global carbon and hydrological cycles. Both systems are considered to be climate tipping elements, characterised by the existence of multiple equilibrium states separated by a critical threshold. Anthropogenic climate change is pushing these systems closer to their respective tipping points, potentially leading to an AMOC slowdown or collapse and a transition of the Amazon from a rainforest to a savanna-like state.

While the AMOC and the ARF have been widely studied separately, their potential interactions remain poorly understood. Rising global temperatures are associated with reduced precipitation over the Amazon and a weakening of the AMOC. These coupled changes suggest two-way interactions, as AMOC weakening can decrease rainfall over the Amazon, while changes in Amazon vegetation can affect AMOC strength, potentially stabilising the climate system or triggering a tipping cascade. In this study, we investigate whether changes in the Amazon Rainforest can influence the stability of the AMOC.
We use the Community Earth System Model (CESM) to perform a set of numerical experiments in which the Amazon region is prescribed with different land-cover states, representing rainforest and grassland conditions. By comparing these experiments, we investigate the climate response to prescribed Amazon vegetation changes and their influence on large-scale atmospheric and ocean circulation.

Our results show that replacing rainforest with grassland leads to a global increase in near-surface air temperature, with the strongest warming occurring over the Amazon region. This transition is associated with pronounced changes in precipitation patterns and atmospheric moisture transport. These findings indicate a potential coupling between Amazon land-cover changes and large-scale climate dynamics, suggesting that Amazon tipping may have implications for AMOC stability.

How to cite: Stanchieri, C., Dijkstra, H. A., Bastiaansen, R., De Maeyer, K., Rietkerk, M., and Staal, A.: The interaction between the Amazon rainforest and the AMOC, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8429, https://doi.org/10.5194/egusphere-egu26-8429, 2026.

EGU26-8560 | Posters on site | ITS4.1/NP8.9

Tipping point analysis of the Scottish peatlands 

Ivan Sudakow, Roxane Andersen, David Large, Andrew Bradley, and Valerie Livina

Satellite data below 100 m resolution can be of great benefit for prevention of geohazards. To utilise spatial and temporal data efficiently, it is necessary to develop data science techniques that are sensitive, computationally light, and capable of revealing signatures of critical events in bulky multivariate data. This emphasis on computationally light yet physically grounded detection aligns with recent climate emulation work that motivates efficient data-driven pipelines for extracting dynamical signatures from large observational datasets [1]. We apply tipping point analysis e.g., Early Warning Indicators (EWS), adapted to multivariate data flows, to demonstrate how this methodology can help complement and augment field work in the peatlands, thus optimising resources.

EWS are based on structural changes in trajectories of dynamical systems, which are described by autocorrelations and variability of the system potential [2-4]. Conventionally, peatlands are studied using expensive and slow ground surveys, but we show that equivalent information can be derived from the satellite Interferometric Synthetic Aperture Radar (InSAR) 6-12 day surface motion data using tipping point analysis. This includes processing the order of hundreds of thousands of time series potentially over 100’s of km, in combination with GIS data provided by stakeholders.

We demonstrate a case study using InSAR surface motion data over ~400km2area in Scotland with areas of critical changes in the soil surface. In a blind test, the area of a large fire (60km2) in Scottish peatlands was identified and its detection coincided with the area of actual fire damage in comparison with ground observations and existing fire detection tools based on MODIS data. This approach is promising and may be developed further to better understand peatland behaviour before and after such extreme events.

References

[1] Sudakow, I., Pokojovy, M., & Lyakhov, D., Statistical mechanics in climate emulation: Challenges and perspectives, Environmental Data Science 1, e16 (2022).

[2] Livina et al., Potential analysis reveals changing number of climate states during the last 60 kyr, Climate of the Past 6, 77-82 (2010)

[3] Livina et al., Forecasting the underlying potential governing the time series of a dynamical system, Physica A, 392 (18), 3891-3902 (2013)

[4] Prettyman et al., A novel scaling indicator of early warning signals helps anticipate tropical cyclones, Europhysics Letters 121, 10002 (2018).

 

How to cite: Sudakow, I., Andersen, R., Large, D., Bradley, A., and Livina, V.: Tipping point analysis of the Scottish peatlands, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8560, https://doi.org/10.5194/egusphere-egu26-8560, 2026.

 

Predicting climate tipping points, such as the collapse of the Atlantic Meridional Overturning Circulation (AMOC), remains a formidable challenge due to the absence of direct observation records of such events and significant parametric and structural uncertainties in Earth System Models (ESMs). It is the grand challenge to explore whether climate tipping or its risk is foreseeable using ESMs and observation without any directs records of climate tipping in the past.

We performed Observation System Simulation Experiments (OSSE) using one of Earth system models of intermediate complexity, LOVECLIM. To assess the predictability of AMOC tipping under a freshwater hosing scenario, we employed a surrogate model-based uncertainty quantification approach to estimate five uncertain parameters related to atmospheric and oceanic physics. We introduced a new dimensionality reduction technique, Wasserstein GEV PCA, which maps the trends of mean climate and extreme events into a flattened statistical manifold using the Wasserstein metric. This allows for the  quantification of observation errors and likelihoods even under transient climate conditions.

Our results demonstrate that while parameters related to precipitation adjustment are critical for accurate AMOC projections, they are difficult to constrain. Comparative analysis reveals that among single-variable observations, Sea Surface Salinity is the most effective constraint for reducing the parametric uncertainty including the precipitation adjustment parameters and narrowing the projection spread of the AMOC. Furthermore, while standard mean-field PCA methods exhibit significant estimation errors when applied to non-stationary data the proposed GEV-based method maintains high robustness and estimation accuracy even with the nonstationary observation. This study highlights that tracking the geometry of extreme value distributions provides a superior pathway for non-stationary climate data, thereby enabling more reliable risk assessments of climate tipping.

How to cite: Kubo, A. and Sawada, Y.: Uncertainty Quantification of an Earth System Model for risk assessment of Climate Tipping via Non-stationary Extreme Events, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9125, https://doi.org/10.5194/egusphere-egu26-9125, 2026.

EGU26-9438 | ECS | Posters on site | ITS4.1/NP8.9

Irreversible Land Carbon Losses under Idealized Overshoot Experiments 

Hyuna Kim, Frerk Pöppelmeier, Benjamin D. Stocker, Urs Hofmann Elizondo, and Thomas L. Frölicher

Terrestrial vegetation and carbon storage may exhibit irreversible responses under anthropogenic climate change and may shift from a carbon sink to a carbon source. Understanding the reversibility of this transition is critical for assessing future carbon-climate feedback. Idealized overshoot experiments provide a controlled framework to test the response of the terrestrial vegetation and its carbon pools to climate forcing. Non-linear responses and incomplete recovery indicate tipping-like behavior. Here, we quantify land carbon changes under idealized overshoot scenarios, following the Tipping Point Model Intercomparison Project (TIPMIP) protocol, employing the LPX Dynamic Global Vegetation Model. We find non-linear responses in land carbon during and after transient warming, as well as recovery behavior. We perform a transient experiment (T1A1 protocol) initialized from pre-industrial conditions (1850) and force LPX with temperature, precipitation, and cloud cover from TIPMIP simulations of the GFDL ESM2M. In the T1A1 protocol, surface air temperature increases linearly by 2 °C over 100 years, remains constant for 50 years, and then decreases by 2 °C over the next 100 years. To assess the long-term recovery in land carbon, we extend the experiment by 1,000 years beyond the T1A1. During the warming phase global total land carbon decreases by about 100 PgC (~5%), comprising losses from vegetation (35 PgC), soil (25 PgC), permafrost (25 PgC), and litter (15 PgC) carbon pools. During the cooling phase back to pre-industrial conditions, approximately 75% of the carbon loss (75 PgC) is restored. The remaining 25% of the deficit reflects a quasi-permanent loss of permafrost carbon associated with warming-induced thaw. Pronounced non-linear responses emerge in northern peatlands, that suggest tipping-like behavior. Ongoing analysis will further constrain the role of hydrology in shaping these responses and their limited reversibility.

How to cite: Kim, H., Pöppelmeier, F., Stocker, B. D., Hofmann Elizondo, U., and Frölicher, T. L.: Irreversible Land Carbon Losses under Idealized Overshoot Experiments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9438, https://doi.org/10.5194/egusphere-egu26-9438, 2026.

EGU26-9785 | ECS | Orals | ITS4.1/NP8.9

Impacts of an AMOC collapse on the North Atlantic jet stream and storm track 

Alejandro Hermoso and Christoph Raible

The Atlantic Meridional Overturning Circulation (AMOC) has a strong influence on global and regional climate. In particular over Europe, previous works have shown that an AMOC tipping to a weak state would lead to a substantial cooling and drying, especially in the high latitudes. In this work, we aim at identifying the impacts of an AMOC collapse to the atmospheric circulation in the North Atlantic by looking at the jet stream and the storm track and link them with changes in the European climate variability and extremes.

We use dynamically downscaled regional climate simulations at 15 km resolution over a 20-year period run with the Weather Research and Forecasting model (WRF). These regional simulations are forced by fully-coupled global runs performed with multiple Earth System models under various prescribed conditions. The experiments consist of a simulation with stable global warming of 2 K and an imposed AMOC collapse on top of the stable global warming. Cyclones are tracked in the WRF simulations and their number, intensity and associated impacts (strong winds and/or heavy precipitation) in the global warming and AMOC collapse experiments are compared to a baseline simulation with pre-industrial forcing. The physical processes leading to the identified changes in the storm track are also studied. This analysis allows us to better understand the modifications in atmospheric dynamics caused by crossing a tipping point and to quantify the subsequent impacts.   

How to cite: Hermoso, A. and Raible, C.: Impacts of an AMOC collapse on the North Atlantic jet stream and storm track, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9785, https://doi.org/10.5194/egusphere-egu26-9785, 2026.

EGU26-10428 | Orals | ITS4.1/NP8.9

Evaluating the skill of a geometric early warning for tipping in a rapidly forced nonlinear system 

Paul Ritchie, Sneha Kachhara, and Peter Ashwin

The future behavioural fate of a forced nonlinear system may at times depend sensitively on the forcing profile as well as natural fluctuations within the system. This is especially the case for rate-induced tipping, where the forcing pushes the system to a basin boundary of a future behaviour and small changes in the forcing can lead to drastically different behaviours. This sensitivity may be present only for a limited time when the forcing is most rapidly changing and so we investigate a geometric early warning to evaluate whether we are in such a sensitive state. This involves computing an approximation of the R-tipping edge state which is a dynamic state that requires knowledge of the future behaviour of the forcing.  We contrast this with early warnings of bifurcation-induced tipping, where an assumption of slow variation of forcing is needed. We provide an example of early prediction of future state for a 3-box model of the Atlantic Meridional Overturning Circulation (AMOC) with specified rapid forcing and show that the skill compares favourably with a simple threshold approach.

How to cite: Ritchie, P., Kachhara, S., and Ashwin, P.: Evaluating the skill of a geometric early warning for tipping in a rapidly forced nonlinear system, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10428, https://doi.org/10.5194/egusphere-egu26-10428, 2026.

Abrupt transitions in the North Atlantic Subpolar Gyre’s (SPG’s) behavior are a major source of uncertainty in decadal-scale climate predictability, as well as having potentially strong impacts on the Atlantic Meridional Overturning Circulation (AMOC), European climate, and marine ecosystems. Climate model simulations suggest that the SPG can undergo irreversible transitions from a regime of deep convection and strong circulation to one characterized by weak convection and reduced transport. Such a collapse would substantially cool the North Atlantic and could interact with a weakening AMOC in complex and nonlinear ways.

SPG transitions emerge from the interplay between high-dimensional ocean dynamics and unresolved stochastic processes, making it difficult to represent them faithfully in current Earth system models and challenging for deterministic prediction frameworks. Here, we use CESM2 pre-industrial control simulations to perform a data-driven analysis of SPG dynamics. We construct a machine-learning-based stochastic neural emulator designed to learn, forecast, and quantify uncertainty in SPG evolution. The model simultaneously learns the conditional mean dynamics and state-dependent ensemble spread, enabling fully probabilistic predictions of key prognostic variables.

This approach provides a tractable framework for investigating the mechanisms and precursors of SPG weakening and deep-convection collapse, and for assessing associated climate risks. When generalized across models, our approach also offers a pathway for systematically evaluating long-timescale North Atlantic dynamics in Earth system simulations.

How to cite: Zhang, H., Ghil, M., and Bouchet, F.: Stochastic neural emulators for subpolar gyre variability and tipping-risk prediction in Earth system models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11528, https://doi.org/10.5194/egusphere-egu26-11528, 2026.

EGU26-12010 | Orals | ITS4.1/NP8.9

On the robustness of Early Warning Indicators 

Bo Christiansen and Shuting Yang

Early warning indicators (EWIs) of tipping points are typically derived from insights gained from simple dynamical systems. Whether these indicators provide robust and reliable warnings when applied to the climate system remains an open question. In this study, we use climate models with known tipping points to investigate the behavior of classical EWIs associated with increasing memory and variance. In addition, we explore an alternative EWI based on changes in spatial correlations.

A key challenge in applying EWIs is determining when a change is significant enough to constitute a warning. How large must a deviation be relative to background variability? How should this background variability be defined—using an early segment of the simulation or an unforced control experiment? How much temporal smoothing should be applied to the indicators? And what is the associated risk of false positives?

We address these questions for several tipping elements, including the Atlantic Meridional Overturning Circulation (AMOC), the subpolar gyre region, and sea ice. Our analysis is based on simulations from both the CMIP6 ensemble and the OptimESM/TipESM ensembles.

Our results indicate that EWIs are generally sensitive to methodological choices and, in some cases, exhibit significant changes only after the tipping point has occurred.

How to cite: Christiansen, B. and Yang, S.: On the robustness of Early Warning Indicators, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12010, https://doi.org/10.5194/egusphere-egu26-12010, 2026.

The Amazon rainforest (ARF) is one of the most important tipping elements on the planet and has been under increasing stress due to global warming and deforestation over the last few decades. Several studies have investigated the stability of the ARF, and the best available estimates indicate that the forest could surpass a tipping point after approximately 25% deforestation or 2–4 °C of global warming. However, there are significant uncertainties surrounding these estimates, and there is still a lack of understanding of how these different forcings (global warming and deforestation) interact and how their combined effects could accelerate a critical transition of large parts of the ARF to a tropical savanna state. In this study, we performed idealized experiments to investigate the hydroclimatic response of the ARF to deforestation-only and composite (global warming + deforestation) forcings, with the aim of better understanding the tipping point potential, how it affects the hydroclimatic stability of the forest, and how the two forcings interact. We therefore performed experiments with 0%, 25%, 50%, 75%, and 100% deforestation under a stable global temperature 2 °C warmer than pre-industrial conditions and analysed the response of four hydroclimatic stress indicators: annual precipitation, dry season length (DSL), mean climatological water deficit (MCWD), and top 10 cm soil moisture. We calculated the deviation of the long-term average of each of these variables from stable (no-deforestation) scenarios and classified the deviations using relative anomalies, defined with respect to the standard deviation of the distribution of the stable scenarios. Using these metrics, an anomaly of 0.5 (i.e., a deviation of the mean by half of the standard deviation of the stable scenario) qualifies as a significant moderate anomaly, while anomalies exceeding 2.0 and 2.5 are classified as severe and extreme anomalies, respectively. We found that deforestation of 25% of the ARF can expose approximately 70% of the rainforest to significant hydroclimatic stress according to at least one of the four indicators analysed. When the combined effects of 25% deforestation and 2 °C of global warming are considered, this fraction increases to 89% of the ARF. This composite effect is larger than the deforestation-only stress resulting from a 50% removal of forest cover (82% of the ARF). Among the indicators, increasing dry season length is the most pronounced response, affecting a larger fraction of the forest and with greater intensity than the other variables, and with effects not limited to the vicinity of deforested areas. Whether tree mortality occurs in areas under significant stress is likely to depend strongly on the ability of the vegetation to rapidly adapt to substantial changes in hydroclimatic conditions. Overall, these results reveal quantitative aspects of the potential for deforestation and global warming to trigger cascading effects in the ARF that could ultimately lead to its transition to a tropical savanna state.

How to cite: Ferreira Correa, L., Bathiany, S., and Pongratz, J.: Amazon rainforest hydroclimatic stress under 2 °C global warming in response to progressive idealized deforestation simulated with MPI-ESM-HR, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12025, https://doi.org/10.5194/egusphere-egu26-12025, 2026.

EGU26-12168 | Posters on site | ITS4.1/NP8.9

TipPFN and TipBox: Early tipping point detection using in-context learning 

Benjamin Herdeanu, Juan Nathaniel, Kai Ueltzhöffer, Carla Roesch, Tobias Weber, Yunus Sevinchan, Vaios Laschos, Gregor Ramien, Johannes Haux, and Pierre Gentine

Climate tipping points emerge from nonlinear feedbacks that can trigger abrupt and potentially irreversible transitions in the Earth system, with far-reaching societal and environmental consequences. Anticipating such critical transitions in complex, high-dimensional systems remains a central challenge. While traditional early-warning indicators rely on assumptions of stationarity, long time series, and simple bifurcation structures. Because these assumptions rarely hold in real data, machine learning approaches have emerged as an alternative, but typically require training data from the specific systems under study, limiting their generalizability.

Here, we present TipBox and TipPFN. TipBox is an open-source, JAX-based repository containing a collection of simple dynamical systems and box models designed for accelerated generation of synthetic data. It enables efficient simulation of deterministic and stochastic systems exhibiting a wide range of bifurcation behaviour such as fold, Hopf, rate- and noise-induced tipping. Since TipBox is differentiable out-of-the-box, it enables easy parameter sensitivity tests for tipping point studies especially when different box models are coupled together.

Building on this synthetic data foundation, we develop TipPFN, a Prior-Data Fitted Network (PFN) approach based on a transformer machine learning architecture that performs approximate Bayesian inference via in-context learning. Trained on carefully selected synthetic dynamical systems, during inference it conditions on a short context of noisy observed data and produces a probabilistic forecast in a single forward pass based on synthetic priors generated from TipBox. This enables fast and computationally cheap probabilistic prediction on systems not seen during training, including time-to-tip as well as the type of tipping point. 

We validate our approach on three systems spanning different domains: an AMOC box model representing climate tipping elements, a predator-prey system from ecology, and a simplified power-grid model from infrastructure research. Preliminary results indicate that our PFN-based predictor generalizes to these complex test cases despite being trained exclusively on the simpler systems in TipBox. Benchmarking against state-of-the-art machine learning approaches shows promising results. We observe improved performance over traditional variance- and autocorrelation-based EWS, particularly under noisy conditions. Ongoing work evaluates conditional probabilistic predictions of the effects of changes in forcing on tipping dynamics.

Overall, we show that TipBox and TipPFN enable robust inference of tipping points on previously unseen systems with models trained purely on synthetic data without the need for additional retraining. This capability is especially powerful for the climate system where direct real-world observations of crucial tipping elements are unavailable but their prior proxies are.

How to cite: Herdeanu, B., Nathaniel, J., Ueltzhöffer, K., Roesch, C., Weber, T., Sevinchan, Y., Laschos, V., Ramien, G., Haux, J., and Gentine, P.: TipPFN and TipBox: Early tipping point detection using in-context learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12168, https://doi.org/10.5194/egusphere-egu26-12168, 2026.

EGU26-12309 | ECS | Posters on site | ITS4.1/NP8.9

Vegetation resilience is linked to moisture availability, temperature, biodiversity and canopy complexity 

Chan Diao, Sebastian Bathiany, Lana L. Blaschke, Subhrasita Behera, Teng Liu, Xiuchen Wu, Pei Wang, Taylor Smith, and Niklas Boers

Assessing the spatial patterns and drivers of terrestrial ecosystem resilience is essential for understanding ecosystem responses to climate change and other environmental pressures. In this study, we investigate global vegetation resilience using long-term solar-induced chlorophyll fluorescence (SIF) observations from two independent satellite products. Resilience is quantified using metrics derived from lag-one autocorrelation  (AC1)  and variance within the framework of critical slowing down theory (CSD). We first evaluate the reliability of SIF-based resilience metrics by comparing them with empirically estimated recovery rates and infer that the SIF datasets are suitable for CSD-based resilience estimates. We further examine how climatic conditions and vegetation structural properties regulate and shape spatial variations in ecosystem resilience. Specifically, we find that water availability and canopy structural complexity show a positive relationship with vegetation resilience, whereas temperature shows a negative relationship with vegetation resilience.  In addition, alpha diversity is positively related to resilience across most vegetation types, although this relationship is weak or absent in grassland ecosystems. These findings confirm the importance of climatic controls while highlighting the combined roles of biodiversity and ecosystem structural complexity in shaping terrestrial vegetation resilience. The resilience spatial patterns and mechanisms identified here provide new insights into ecosystem stability under ongoing climate change.

How to cite: Diao, C., Bathiany, S., Blaschke, L. L., Behera, S., Liu, T., Wu, X., Wang, P., Smith, T., and Boers, N.: Vegetation resilience is linked to moisture availability, temperature, biodiversity and canopy complexity, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12309, https://doi.org/10.5194/egusphere-egu26-12309, 2026.

EGU26-12673 | ECS | Posters on site | ITS4.1/NP8.9

Amazon tipping advances and amplifies biodiversity loss through teleconnected precipitation declines 

Clemens Giesen, Maximilian Kotz, Nico Wunderling, Damaris Zurell, and Leonie Wenz

The Amazon rainforest is the most species-rich region on Earth, being home to approximately ten percent of all species worldwide. However, human influences such as global warming, deforestation, and land-use change are placing unprecedented pressure on the rainforest, endangering this unique ecosystem. Recent findings suggest that the Amazon rainforest could cross a tipping point within this century when deforestation and climate change are considered together. In this study, we project the impact of such a potential tipping point on the biodiversity of the Amazon basin and compare it with a scenario without tipping. To do so, we use climate data generated by a dynamical tipping point model which simulates the Amazon forest system using a moisture-recycling network under different climate and deforestation scenarios. To assess the impact on species we compare changes in climatically suitable areas for nearly 2,000 species in the Amazon basin using an ensemble of species distribution models. Our results show that the combined effect of deforestation and climate change leads to a substantially stronger decline in climatically suitable areas than climate change alone. Including deforestation results in markedly intensified biodiversity losses already early in the century (2030-2044). Notably, the largest differences in species richness loss between scenarios do not occur in deforested area but several hundred kilometres away. These teleconnected losses are driven by deforestation-induced disruptions of atmospheric moisture transport, causing precipitation declines in distant regions and pushing species beyond their climatic niches. Overall, our results indicate that limiting global warming together with halting deforestation is critical to preventing severe and widespread biodiversity losses in the Amazon within the coming decades.

How to cite: Giesen, C., Kotz, M., Wunderling, N., Zurell, D., and Wenz, L.: Amazon tipping advances and amplifies biodiversity loss through teleconnected precipitation declines, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12673, https://doi.org/10.5194/egusphere-egu26-12673, 2026.

EGU26-14181 | ECS | Posters on site | ITS4.1/NP8.9

Sahara and boreal forests natural vegetation: from mid-Holocene to future 

Charline Ragon, Pascale Braconnot, and Olivier Marti

As anthropogenic forcing increases, there is a rising concern about crossing tipping points. A key information is the critical thresholds at which the so-called tipping elements could undergo abrupt changes, and the associated early-warning signals. This is true, in particular, for boreal forests and the possible greening of the Sahara. In that perspective, testing climate models against paleoclimate allows for exploring the climate response over multi-millennial time series, while offering the possibility to compare it with past vegetation reconstructions.

We consider a transient simulation from the mid-Holocene (6,000 years before present) to 2100 obtained using the IPSL general circulation model including dynamical natural-only vegetation [1]. The simulation is forced with changes in orbital parameters and trace gases, transitioning from the paleo- to the historical period, and then to the scenario SSP4.5. We focus on two terrestrial ecosystems, both identified as tipping elements: the Sahara/Sahel and boreal forests in northern Europe.

We analyze the evolution of vegetation patterns and extents in the two regions along the Holocene with the objective to determine if their response to forcing conditions can be assimilated to the crossing of a tipping point. Thus, we isolate rapid shifts and investigate whether they correspond to tipping points or to centennial variability. We link them to changes in regional vegetation drivers, including vegetation feedbacks, or to AMOC variability. Then, we explore possible analogies between changes during the Holocene and in projections, allowing for the identification of sensitive regions, which may help to detect regional thresholds for tipping points.

References:

[1] Braconnot, P., Viovy, N., and Marti, O. (2025). Dynamic vegetation highlights first-order climate feedbacks and their dependence on climate mean state. Earth System Dynamics, 16, 2113–2136.

How to cite: Ragon, C., Braconnot, P., and Marti, O.: Sahara and boreal forests natural vegetation: from mid-Holocene to future, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14181, https://doi.org/10.5194/egusphere-egu26-14181, 2026.

EGU26-14948 | ECS | Posters on site | ITS4.1/NP8.9

Satellite-based Tracking of Resilience Change in South American Tropical Dry Forests 

Anton Schulte-Fischedick, Teng Liu, Lana Blaschke, Taylor Smith, Sebastian Bathiany, Niklas Boers, and Tobias Kuemmerle

Tropical dry forests are important for biodiversity and people, yet also exposed to high pressure from agricultural expansion and climate change, raising concerns about declining forest resilience. Global analyses of forest resilience have revealed a widespread loss of resilience in tropical and arid forests, as well as declining and increasingly more variable rainfall in many tropical regions. However, tropical dry forests have so far not been explicitly focused on in assessments of resilience under climate and land-use change. A key limitation of existing studies, which have predominantly relied on MODIS-based proxies such as the Normalised Difference Vegetation Index or VODCA-based vegetation optical depth, is that the comparatively coarse spatial resolution of these sensors cannot adequately resolve and analyse small-scale resilience changes in tropical dry forests, which are characterised by high compositional and structural heterogeneity.

Here, we address these gaps and track changes in the resilience of South American tropical dry forests using the high-resolution Landsat archive since 1999. We derive vegetation resilience trends using robust regression based on temporal and spatial indicators of critical slowing down of kNDVI time series. Additionally, we explore how local resilience trends are associated with accessibility and land use gradients, such as distances to roads, cities, and agricultural areas, as well as the hydrological context, such as distances to water surfaces. Our results show distinct patterns of resilience change in South American tropical dry forests. Nonetheless, substantial uncertainties in resilience tracking using the Landsat archive remain due to sensor inconsistencies and missing data.

How to cite: Schulte-Fischedick, A., Liu, T., Blaschke, L., Smith, T., Bathiany, S., Boers, N., and Kuemmerle, T.: Satellite-based Tracking of Resilience Change in South American Tropical Dry Forests, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14948, https://doi.org/10.5194/egusphere-egu26-14948, 2026.

EGU26-15745 | ECS | Posters on site | ITS4.1/NP8.9

Widespread vulnerable greening of terrestrial vegetation in a warming world 

Mengya Zhao, Yulin Shangguan, and Zhou Shi

Terrestrial vegetation has continued to green in recent decades under warming and rising atmospheric CO2, yet ecosystem resilience has declined across large portions of the globe. The extent, spatial patterns, and drivers of this emerging decoupling between vegetation greening and resilience remain poorly understood. Here, we assess the dynamics of vegetation greenness and resilience, and disentangle the underlying mechanisms that drive their emerging decoupling using multiple satellite-derived and modelled data. We show that a pervasive pattern of vulnerable greening, characterized by increasing greenness but declining resilience, affects 41.5% of global vegetated land. This pattern is primarily driven by recent changes in temperature and water availability, which exert distinct impacts on vegetation greenness and resilience. Rising temperature generally enhances vegetation greening, but leads to a persistent decline in resilience, especially in tropical and boreal forests. Variability in water availability dominates resilience loss over 23.0-42.1% of vulnerable greening area across vegetation types, whereas its influence on greenness is negligible. Current Earth system models fail to capture the resilience dynamics, yielding systematically underestimated resilience but overly optimistic trends. Our findings reveal a pervasive hidden erosion of ecosystem stability beneath the apparent greening, highlighting growing risks to the terrestrial carbon sink, and the urgent need to better represent vegetation resilience in climate-change assessments.

How to cite: Zhao, M., Shangguan, Y., and Shi, Z.: Widespread vulnerable greening of terrestrial vegetation in a warming world, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15745, https://doi.org/10.5194/egusphere-egu26-15745, 2026.

EGU26-16364 | ECS | Orals | ITS4.1/NP8.9

AI emulator highlights underestimated risk of AMOC collapse in current climate models 

Yechul Shin, Niklas Boers, Yu Huang, Bahar Emirzade, Jiho Ko, Ji-Hoon Oh, and Jong-Seong Kug

The pivotal role in regulating the global climate system and the potential for irreversible collapse underscore the critical importance of the Atlantic Meridional Overturning Circulation (AMOC) and its stability. To address the inherent nonlinearity and stochastic nature of the AMOC, we develop a Convolutional Neural Network (CNN) model to project AMOC evolution using atmospheric and oceanic climate model inputs. Our CNN model successfully captures the stochastic AMOC bifurcation present in large-ensemble climate model simulations. Using explainable AI, we find that the salinity structure enables the CNN to predict future AMOC trajectories, suggesting that the salt-advection feedback amplifies subtle perturbations. Current climate models systematically misrepresent this salinity structure. We show that correcting these biases shifts the climate model projections towards a collapse-prone regime, implying that the AMOC’s stability in current climate models is likely overestimated. Our findings suggest that the risk of AMOC collapse cannot be ruled out simply based on model projections, calling for more thorough investigations of AMOC stability with focus on potential stability biases in climate models.

How to cite: Shin, Y., Boers, N., Huang, Y., Emirzade, B., Ko, J., Oh, J.-H., and Kug, J.-S.: AI emulator highlights underestimated risk of AMOC collapse in current climate models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16364, https://doi.org/10.5194/egusphere-egu26-16364, 2026.

EGU26-16548 | ECS | Posters on site | ITS4.1/NP8.9

Data-driven sequential analysis of tipping in high-dimensional complex systems 

Tomomasa Hirose and Yohei Sawada

Detecting tipping points in the Earth system is a significant challenge, particularly given the high dimensionality, observational sparsity and noisiness in real climatological data. Even in the most classical Bifurcation-induced tipping(B-tipping) with quasi-static forcing, conventional Early Warning Signals based on Critical Slowing Down often struggle with these complexities and can yield false positives in non-tipping scenarios. To address these limitations, we propose a tipping analysis indicator:  High-dimensional Attractor’s Structural Complexity (HASC).

From reconstructed high-dimensional states from partial observations, we extract geometrical structures of trajectories using manifold learning method based graph approximation (Uniform Manifold Approximation and Projection) but without dimension reduction. We quantify the time-evolution of the system's structural complexity using the spectral property of the graph Laplacian, Von Neumann Entropy.

We show that HASC serves as a warning indicator of structural degeneracy of trajectory on 3box AMOC tipping model in B-tipping setting, and analyze further applications against N-and R-tipping. We also demonstrate its application to a realistic CESM AMOC collapse simulation (+10,000 dimensions). This approach offers a training-free, multivariate, and geometry-aware tool for monitoring regime shifts in complex systems.

How to cite: Hirose, T. and Sawada, Y.: Data-driven sequential analysis of tipping in high-dimensional complex systems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16548, https://doi.org/10.5194/egusphere-egu26-16548, 2026.

EGU26-17081 | Posters on site | ITS4.1/NP8.9

Early Warning of Ocean Tipping Points: A Deep Learning model approach 

Thomas Prime and Bablu Sinha

In the study of nonlinear dynamics, tipping points have been a major focus of research. They describe a threshold where gradual changes in external forcing, e.g. increasing CO2 emissions can lead to an abrupt and persistent transition. This is a concern in ocean sciences due to the strong coupling of the ocean and climate. The capability to provide an early warning of a tipping element is desirable, providing time to mitigate and adapt.

Specific regions of the ocean are of more concern for potential tipping elements than others, a key region being the sub polar gyre. This is a basin-scale cyclonic gyre in the North Atlantic, driven by wind and buoyancy forcing. It is crucial in the formation of North Atlantic Deep Water, a main contributor to the lower branch of the Atlantic Meridional Overturning Circulation (AMOC). If this deep convection process collapses, then cascading changes in sea ice, atmospheric circulation, ocean circulation and sea level, and the terrestrial ecosystem are expected.

Machine Learning approaches suggest that a generalised deep learning (DL) model could potentially provide a robust and high confidence solution to predicting tipping points. We have applied an existing generalised DL model to a large ensemble of historical and future climate projections (1950-2100) based on the HadGEM3 Atmosphere-Ocean-Sea-Ice-Land model under the SSP370 future shared socioeconomic pathway scenario. Using change point analysis to identify tipping points in this ensemble, the DL was provided with timeseries of several parameters, leading up to but not including the identified tipping points.  We then assessed the ability of the DL to predict the tipping points based on the chosen parameter timeseries across a number of specific geographic regions.

Mixed Layer Depth and Sea Surface Height were the most effective parameters and there was a large variation in the effectiveness across different regions, with some (Labrador Sea) being much better than others (Irminger Sea). While current DL models are not yet capable of robust tipping point detection there is clear promise in continuing to refine this method with new DL models specifically created for ocean surface and subsurface parameters, such as MLD and temperature and salinity depth profiles.

How to cite: Prime, T. and Sinha, B.: Early Warning of Ocean Tipping Points: A Deep Learning model approach, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17081, https://doi.org/10.5194/egusphere-egu26-17081, 2026.

EGU26-17794 | Orals | ITS4.1/NP8.9

Stability landscapes: evidencing critical slowing down and ecological resilience in grassland ecosystems 

Daniel Simms, Will Rust, Marko Stojanovic, James Bullock, Ron Corstanje, and Jim Harris

Critical slowing down has been proposed as an early warning signal for critical transitions in ecosystems (tipping points) and for defining ecological resilience. However these concepts are difficult to define in ecological systems, which limits how they can be used operationally for advanced warning of changes in ecosystem function and composition. Here we use dense time-series satellite measurements of vegetation productivity in UK grasslands, combined with a dynamic linear model, to estimate ecosystem speed and construct stability landscapes: potential-like surfaces that quantify the geometry governing transitions in response to major droughts that provide empirical evidence for resilience concepts in real-world ecosystems. We anticipate the use of our approach to better understand and visualize ecosystem resilience and as a tool for identifying ecosystems in critical transition that can be targets for intervention, such as ecological restoration.

How to cite: Simms, D., Rust, W., Stojanovic, M., Bullock, J., Corstanje, R., and Harris, J.: Stability landscapes: evidencing critical slowing down and ecological resilience in grassland ecosystems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17794, https://doi.org/10.5194/egusphere-egu26-17794, 2026.

EGU26-18199 | ECS | Orals | ITS4.1/NP8.9

Detecting Abrupt Shifts and Coherent Spatial Domains in Earth System Data with TOAD  

Jakob Harteg, Lukas Röhrich, Kobe De Maeyer, Julius Garbe, Boris Sakschewski, Ann Kristin Klose, Jonathan Donges, Ricarda Winkelmann, and Sina Loriani

We present TOAD v1.0 (Tipping and Other Abrupt events Detector), an open-source Python framework for the systematic detection and analysis of abrupt shifts in gridded Earth system data. TOAD provides a user-oriented workflow that combines grid-level shift detection with spatio-temporal clustering to identify domains where abrupt change co-occurs. An optional ensemble consensus step then identifies spatial patterns that are robust across ensemble members, models, variables, or method configurations, and quantifies associated statistics. The framework is method-agnostic, allowing different detection and clustering algorithms to be compared within a reproducible analysis pipeline. TOAD serves as an introspection tool for exploratory analysis of abrupt change across scales and addresses key questions in tipping-point research by identifying where such changes occur and providing first-order information on when they emerge along a time or forcing trajectory. The framework supports coordinated analyses in large model ensembles and intercomparison projects, such as TIPMIP and CMIP.

How to cite: Harteg, J., Röhrich, L., De Maeyer, K., Garbe, J., Sakschewski, B., Klose, A. K., Donges, J., Winkelmann, R., and Loriani, S.: Detecting Abrupt Shifts and Coherent Spatial Domains in Earth System Data with TOAD , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18199, https://doi.org/10.5194/egusphere-egu26-18199, 2026.

EGU26-18335 | ECS | Posters on site | ITS4.1/NP8.9

Scale Dependence of Spatial Patterns and Tipping Dynamics in the Boreal Forest 

Cesar Murad, Jadu Dash, John Dearing, Neil Brummitt, and Felix Eigenbrod

Escalating climate extremes and environmental pressures are increasingly pushing ecosystems toward regime shifts across the biosphere. Before tipping, however, ecosystems typically lose resilience and exhibit slower recovery from perturbations. This “critical slowing down” behaviour can be quantified through statistical measures to detect early warning signals (EWSs) that arise in timeseries as rising variance, autocorrelation, and skewness. In the spatial domain, the emergence of regular vegetation patterns, known as Turing patterns, has been proposed as a spatial EWS that, along with increasing spatial variability, is interpreted as a hallmark of an approaching critical transition. Nonetheless, a broader gradual spatial reorganisation may instead reflect an ecosystems potential to avoid abrupt collapse by undergoing a Turing bifurcation, experiencing progressive changes in resilience while still drifting towards a less desirable alternative regime. These contradictory theories of what EWSs mean for ecosystems make it crucial to assess whether spatial variability in vegetation emerges as a distinctive sign of an ecosystems’ change in resilience following non-catastrophic shifts. We apply a theoretically grounded framework that links alternative tipping archetypes, such as fold and Turing bifurcations, to expected signatures in both temporal and spatial indicators. By comparing the observed multiscale spatiotemporal patterns with the expectations of different tipping archetypes, we aim to disentangle the scale dependence of tipping dynamics to identify the dominant forcing-response mechanisms operating in complex terrestrial ecosystems. Among these, the Canadian boreal forest stands as a crucial carbon stock exposed to rapid and pronounced warming that renders it vulnerable to structural and compositional transformation. Monitoring it is therefore essential to improve our understanding of the underlying physical mechanisms driving vegetation dynamics and addressing the potential impacts on the ecosystem services they provide if transitioning into degraded states. To achieve this, satellite derived vegetation indices were employed to quantify spatial patterns across multiple resolutions, using hexagonal discrete global grids to characterise vegetation changes in resilience and spatial structure through time. Within a case study region in northern Quebec, the boreal forest exhibited a greening trend from 1984 to 2022 evidenced by an increasing mean of the vegetation indices across scales, but, with an overall decreasing trend in spatial autocorrelation and contrasting trends in spatial variance throughout the region. The observed trends were predominantly prominent at the forest community scales, suggesting a potential scale dependence of the operating tipping archetype and its associated EWS metrics. Datasets on climatic drivers and catastrophic disturbances, including wildfires, droughts, pathogen, and insect outbreaks, are further incorporated to distinguish exogenous forcing from endogenous ecosystem responses and feedbacks. Identifying these could elucidate whether gradual spatial reorganisation or an impending critical transition in vegetation is occurring. The outcomes could further provide actionable insights to support and improve the management, restoration, and mitigation strategies for forested ecosystems under accelerating climate change.

How to cite: Murad, C., Dash, J., Dearing, J., Brummitt, N., and Eigenbrod, F.: Scale Dependence of Spatial Patterns and Tipping Dynamics in the Boreal Forest, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18335, https://doi.org/10.5194/egusphere-egu26-18335, 2026.

EGU26-18498 | ECS | Orals | ITS4.1/NP8.9 | Highlight

To tip or not to tip 

Reyk Börner and Henk A. Dijkstra

Tipping points have become a buzzword in earth system science. The more popular the term becomes, the less clear its definition seems. While for some a tipping point is simply a metaphor of something changing quickly, others mean a bifurcation threshold in a strict mathematical sense. Also the Intergovernmental Panel on Climate Change has struggled defining tipping, relying on challenging notions such as abruptness and irreversibility. However, agreeing on what tipping means, and whether a system tips or not, is important both for robust science as well as for communicating climate tipping risk to policymakers and the public.

Here we critically evaluate the problems with existing tipping definitions. Based on this, we propose a revised definition that characterizes tipping behavior as a nonlinear transition in forced systems. Our definition emphasizes both the phenomenology (observed time series) and cause (feedback mechanism) of a tipping event. While compatible with dynamical systems theory, our proposition avoids concepts such as bifurcations or equilibrium states, making the definition applicable also to transient dynamics in highly complex systems under time-varying forcing. We showcase its practical use in case studies of earth system model data, comparing slow tipping systems (e.g. ice sheets) with fast tipping systems (e.g. tropical rainforests).

How to cite: Börner, R. and Dijkstra, H. A.: To tip or not to tip, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18498, https://doi.org/10.5194/egusphere-egu26-18498, 2026.

EGU26-20397 | Posters on site | ITS4.1/NP8.9

Investigating Greenland Ice Sheet tipping in the Tipping Points Modeling Intercomparison Project (TIPMIP) 

Donovan Patrick Dennis, Torsten Albrecht, Shivani Ehrenfeucht, Ann Kristin Klose, Leonie Reontgen, and Ricarda Winkelmann

Understanding the potential future evolution of the Greenland Ice Sheet (GrIS) is of critical importance for anticipating the consequences of global climate change. GrIS melt contributes between 0.5-0.8 mm per year to total global sea level rise and the total ice volume has the potential to raise sea levels by 7 meters. Furthermore, freshwater delivery to the North Atlantic has important implications for the stability of the density-driven Atlantic Meridional Overturning Circulation. A critical challenge in anticipating GrIS sea level rise contribution and North Atlantic freshwater delivery arises from the so-called inertia of the ice sheet, wherein present-day and near-term future warming may trigger ice loss that unfolds on century to millennial timescales. The GrIS is considered one of the Earth system’s tipping elements, components of the Earth system wherein crossing a critical global warming threshold leads to large-scale and nonlinear change in system state. Though it is subject to a number of self-amplifying (and -dampening) feedbacks, the susceptibility of the GrIS to tipping is not well-constrained, with particular uncertainties arising over long (1-10 kyr) timescales, given different global warming rates, and under potential scenarios of “stabilised” or landing climate (i.e., the Paris-agreed 1.5 C). 

 

The Tipping Points Modelling Intercomparison Project (TIPMIP) seeks to investigate the likelihood, impacts, and risk of crossing Earth system tipping points in so-called global tipping elements—components which, if tipped, have widespread consequences for the whole Earth system. Here we present initial explorations of the response of the GrIS to the transient, idealised warming scenarios following the TIPMIP-ESM and TIPMIP-ICESHEET domain protocols, with standalone, offline experiments undertaken using the Parallel Ice Sheet Model (PISM). These idealised warming scenarios have been designed to explore both the warming-induced triggers of tipping dynamics as well as their feedbacks over century to millennia timescales.

How to cite: Dennis, D. P., Albrecht, T., Ehrenfeucht, S., Klose, A. K., Reontgen, L., and Winkelmann, R.: Investigating Greenland Ice Sheet tipping in the Tipping Points Modeling Intercomparison Project (TIPMIP), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20397, https://doi.org/10.5194/egusphere-egu26-20397, 2026.

EGU26-20432 | ECS | Orals | ITS4.1/NP8.9

Early warning signals and tipping behaviour in Greenland’s glacier periphery from large forcing ensembles 

Larissa Nora van der Laan, Ruth Rhiannon Chapman, Peng Gu, Victor Elvira, and Andrea Quintanilla

The cryosphere is considered a potential tipping element of the Earth system, yet identifying critical thresholds and early warning signals remains challenging due to the computational cost of high-complexity ice-sheet models. Here, we investigate tipping behaviour in the glacier periphery of Greenland using the Open Global Glacier Model (OGGM), exploiting its efficiency to explore a wide range of climate forcing scenarios.

We perform a large ensemble of simulations driven by (i) standard future climate scenarios up to 2100, (ii) scenario-neutral climate trajectories, and (iii) additional physically realistic and idealized forcing experiments. This ensemble approach enables systematic exploration of glacier responses across a broad forcing space, including regimes not typically sampled by comprehensive ice-sheet models. We analyze the resulting time series of glacier volume, area and mass balance for early warning signals of critical transitions, focusing on indicators of critical slowing down such as increasing variance and autocorrelation.

By comparing the emergence and robustness of these signals across forcing types, we assess whether abrupt and potentially irreversible retreat of peripheral Greenland glaciers is preceded by detectable changes in system dynamics. We further identify climatic thresholds and boundary conditions under which tipping-like behaviour is most likely to occur.

Our results aim to provide physically grounded constraints on critical forcing levels relevant to Greenland’s glacier periphery and to inform ice-sheet modelling efforts by highlighting regions of parameter space where nonlinear responses are expected. This work demonstrates the value of intermediate-complexity glacier models for advancing the detection and interpretation of tipping points and early warning signals in the cryosphere.

How to cite: van der Laan, L. N., Chapman, R. R., Gu, P., Elvira, V., and Quintanilla, A.: Early warning signals and tipping behaviour in Greenland’s glacier periphery from large forcing ensembles, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20432, https://doi.org/10.5194/egusphere-egu26-20432, 2026.

EGU26-21078 | ECS | Posters on site | ITS4.1/NP8.9

Impacts of the Subpolar Gyre weakening on European climate extremes  

Valeria Mascolo, Reinhard Schiemann, and Andrea Dittus
Abrupt changes in North Atlantic ocean circulation are among the most critical potential tipping points in the Earth system, with far-reaching implications for European climate extremes. This study investigates the potential weakening and collapse of the Subpolar Gyre using simulations from the UK Earth System Model, testing different definitions and examining outcomes across multiple levels of global warming. It assesses how such a shift could change the frequency and spatial patterns of temperature and precipitation extremes across Europe.
 
The preliminary analysis focuses on characterising the onset of Subpolar Gyre weakening and the feedback mechanisms that shape its evolution, as well as evaluating downstream impacts on regional heatwaves and cold spells. By linking large-scale ocean tipping dynamics to European climate impacts, this work aims to improve understanding of the cascading effects of climate change–driven tipping points on climate extremes. The study also underscores the need for integrated assessments that connect physical tipping elements with adaptation and resilience planning in Europe.

How to cite: Mascolo, V., Schiemann, R., and Dittus, A.: Impacts of the Subpolar Gyre weakening on European climate extremes , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21078, https://doi.org/10.5194/egusphere-egu26-21078, 2026.

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