Presentation type:
GI – Geosciences Instrumentation & Data Systems

EGU25-21957 | Orals | MAL12-GI

Microwave tomography for subsurface prospecting 

Francesco Soldovieri

Ground Penetrating Radar (GPR) is a diagnostic tool that well assessed in a variety of areas, including geophysics, archaeological prospection, civil engineering, and planetary exploration, just to mention few examples.

Notwithstanding the simplicity of the underlying principle, a significant limitation of GPR is concerned with the interpretability of the raw data, mostly presented under the form of radargrams, particularly in scenarios that are complicated and characterised by a multitude of embedded targets. 

To enhance the interoperability of radar images, it is crucial to reliably model the electromagnetic scattering, so that the radar imaging is conceptualised as an inverse scattering problem. For such an inverse problem, the geometric and electromagnetic properties of the targets are retrieved by the field scattered by the target when an incident field impinges on it. Despite the simplicity of the underlying principle, this inverse problem is inherently complex due to its non-linear nature and ill-posedness. These mathematical difficulties have a detrimental effect on the effectiveness of GPR diagnostics in real cases. To facilitate the application of inverse scattering approaches in real-world scenarios, it is necessary to resort to approximate models of electromagnetic scattering. Microwave tomography exploits the linearization of the inverse scattering problem, so that reconstruction approaches can be developed that operate under realistic conditions with the aim of estimating the position and geometry of targets, albeit with limitations on the class of unknowns that can be reconstructed (i.e. resolution limitations) and the impossibility of quantitatively estimating the electromagnetic properties of targets.

In the talk, microwave tomography will presented under a unified mathematical framework based on the solution of an integral equation accounting for arbitrary measurement configurations and background scenarios for both contact and contactless GPR measurements. Furthermore, the investigation of the reconstruction performance of the microwave tomographic approach for different measurement configurations and background scenarios will be presented.

Finally, several cases of exploitation of the microwave tomographic approach in real cases will be shown.

How to cite: Soldovieri, F.: Microwave tomography for subsurface prospecting, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21957, https://doi.org/10.5194/egusphere-egu25-21957, 2025.

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

A Novel Q-Switch Technique for  Borehole NMR Measurement 

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

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

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

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

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

EGU25-4077 | ECS | Posters virtual | VPS19

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

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

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

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

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

EGU25-4641 | Posters virtual | VPS19 | Highlight

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

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

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

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

EGU25-7004 | Posters virtual | VPS19

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

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

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

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

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

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

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

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

EGU25-7921 | ECS | Posters virtual | VPS19

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

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

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

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

 

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

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

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

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

EGU25-13330 | ECS | Posters virtual | VPS19

Advancing and Supporting FAIR Principle Adoption through Innovative Social Infrastructure Tools 

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

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

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

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

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

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

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

EGU25-13917 | ECS | Posters virtual | VPS19

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

Yuanzhi Cai, Ryan Manton, and Morgan Williams

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

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

EGU25-14821 | ECS | Posters virtual | VPS19

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

Deepayan Chakraborty and Adway Mitra

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

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

EGU25-14839 | ECS | Posters virtual | VPS19

Leveraging MAUNet for Bias Correction of TRMM Precipitation Estimates 

Sumanta Chandra Mishra Sharma and Adway Mitra

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

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

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

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

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

EGU25-15216 | Posters virtual | VPS19

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

Graziella Emanuela Scarcella, Luigi Aceto, and Giovanni Gullà

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

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

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

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

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

EGU25-15381 | ECS | Posters virtual | VPS19

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

Maisnam Nongthouba, Bakimchandra Oinam, and Khwairakpam Sachidananda

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

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

EGU25-16092 | Posters virtual | VPS19

Transforming GNSS Data into FAIR Digital Objects 

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

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

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

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

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

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

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

Hybrid Machine Learning approach for Tropical Cyclones Detection 

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

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

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

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

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

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

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

 

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

 

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

 

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

 

Acknowlegments

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

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

EGU25-16634 | Posters virtual | VPS19

Finetuning and Benchmarking an AI Foundation Model for Cloud Gap Imputation  

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

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

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

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

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

 References

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

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

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

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

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

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

EGU25-18822 | Posters virtual | VPS19

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

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

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


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

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

EGU25-18933 | Posters virtual | VPS19

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

Harsha Vardhan Kaparthi and Alfonso Vitti

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

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

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

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

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

EGU25-19489 | ECS | Posters virtual | VPS19

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

Asma Slaimi and Michael Scriney

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

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

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

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

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

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

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

EGU25-20324 | ECS | Posters virtual | VPS19

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

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

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

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

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

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

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

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

EGU25-20616 | ECS | Posters virtual | VPS19

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

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

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

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

EGU25-21759 | Posters virtual | VPS19

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

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

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

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

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

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

EGU25-2237 | Posters virtual | VPS20

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

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

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

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

EGU25-4994 | ECS | Posters virtual | VPS20

bibliometric analysis of natural lakes and paleolakes origin of natural events 

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

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

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

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

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

EGU25-5359 | ECS | Posters virtual | VPS20

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

Jonelle Sayama and Keanno Fausto

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

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

EGU25-6240 | ECS | Posters virtual | VPS20

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

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

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

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

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

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

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

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

EGU25-8063 | ECS | Posters virtual | VPS20

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

Keanno Fausto and Jonelle Sayama

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

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

EGU25-11808 | ECS | Posters virtual | VPS20

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

Pietro Belba

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

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

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

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

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

DISCUSSION AND CONCLUSIONS

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

KEY-WORDS

InSAR, DInSAR, Interferogram

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

EGU25-12947 | ECS | Posters virtual | VPS20

Topological fingerprinting of dynamical systems 

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

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

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

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

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

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

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

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

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

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

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

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

EGU25-15569 | Posters virtual | VPS20

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

Jorge Mendes and Marc Portier

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

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

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

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

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

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

EGU25-16203 | ECS | Posters virtual | VPS20

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

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

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

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

EGU25-17156 | Posters virtual | VPS20

Leveraging EO for Security and Resilience 

Michela Corvino and the Michela Corvino

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

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

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

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

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

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

EGU25-17965 | ECS | Posters virtual | VPS20

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

Daniel Vacca, Borja Aguiar-González, and Tammy Morris

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


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


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

 

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

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

EGU25-18606 | ECS | Posters virtual | VPS20

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

Shivam Kasture, Aishwarya Hegde A, and Pruthviraj Umesh

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

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

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

EGU25-19070 | Posters virtual | VPS20

Rainfall Dynamics in Wind Energy Scenarios 

Martin Obligado and Auguste Gires

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

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

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

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

EGU25-19225 | Posters virtual | VPS20

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

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

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

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

EGU25-20653 * | Posters virtual | VPS20 | Highlight

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

Shaun Lovejoy, Andrej Spiridonov, and Lauras Balakauskas

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

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

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

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

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

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

GI1 – General sessions on geoscience instrumentation

EGU25-176 | Orals | GI1.1

Universal photo-electronic level sensor 

Misha Krassovski, Thomas Shaddix, Gavin Long, Lloyd Clonts, and Nance Ericson

A wide range of industry and scientific applications require continuous measurement of granular or liquid material levels. For environmental science, these include snow depth, water level, and soil erosion measurements. The modern market offers many different sensors, some of which can be used for these measurements, but many of them are expensive and not autonomous. Current market models also propose difficulties in organizing scalable measurement campaigns and limit coverage of large areas. For example, common snow depth and water level sensors are ultrasonic, which requires substantial power, a datalogger, $1000 cost, special mounting, and provides only a single point measurement. This immediately presents itself as both a problematic and expensive route when trying to organize observations across a large area, such as with snow distribution and redistribution. We present Universal photo-electronic level sensor that can be used to measure changes in levels of a media measuring amount of light received by exposed and covered parts of sensor. The intended use are snow depth, water level, and soil erosion measurements.

How to cite: Krassovski, M., Shaddix, T., Long, G., Clonts, L., and Ericson, N.: Universal photo-electronic level sensor, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-176, https://doi.org/10.5194/egusphere-egu25-176, 2025.

EGU25-1913 | ECS | Orals | GI1.1

Storm detection in the North sea with a subsea telecommunication cable and State of Polarization sensing 

Julián Pelaez, Steinar Bjørnstad, and Peter James Thomas

Fibre-optic sensing (FOS) techniques have gained notoriety for geoscientific and industrial applications over the past years. While most research tends to focus on spatially distributed techniques (e.g. Distributed Acoustic/Vibration Sensing), here we investigate the use of State of Polarization (SoP) sensing for ocean observation. SoP is a technique that samples spatially-integrated measurements remotely, i.e. the net change in polarization of light between the ends of an optical fibre link up to hundreds of kilometers long, which can be affected by mechanical strains on one or more sections of the fibre.

We present statistical analyses of an 11-month data set of a continuous SoP recording on a 150 km-long subsea telecommunication cable that crosses the southwestern Norwegian trench between Egersund (Norway) and a shallow (<100 m) FPSO (Floating production storage and offloading) platform on the Eigersunds bank. Our system measures net variations of the S1 Stokes parameter of polarized laser beam injected into the fibre. We observe North sea storms represented in SoP measurements as prominent anomalies with well-defined temporal and spectral features that are consistent with surface gravity wave anomalies. These events are confirmed by comparison with both, hourly ocean wave analysis numerical model time series (0.05° grid resolution) and simultaneous oceanographic measurements at locations adjacent to the cable.

Preliminary results show linear regression coefficients of determination of up to nearly 70% between rms SoP values and modeled significant wave height anomalies above 1 m at frequencies between 0.035-0.56 Hz. Remarkably, variations in the correlation statistics are found as a function of wave propagation direction, which could potentially allow for the discrimination of storms with variable azimuthal properties for a given cable link interrogated with SoP.

We highlight the value of these measurements for in-situ sea state monitoring. Although SoP systems effectively average-out all measurable signals along the entire sensed link, require access to two cable ends (or looped fibres) and are comparatively less sensitive than distributed FOS techniques, they also offer advantages over the latter as well as over established oceanographic sensors due to its relative low cost, sensor simplicity, large coverage, inherent remote data transmission, and relaxed data management requirements.

How to cite: Pelaez, J., Bjørnstad, S., and Thomas, P. J.: Storm detection in the North sea with a subsea telecommunication cable and State of Polarization sensing, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1913, https://doi.org/10.5194/egusphere-egu25-1913, 2025.

EGU25-3145 | Orals | GI1.1

New Echoes Compact Sub-Bottom Profiler (SBP): Portable SBP for inland & coastal environments 

Guillaume Jouve, Emmanuel Chapron, and Brocard Gilles

A significant part of paleoclimate/paleoenvironmental-related geoscience research involves high-resolution sedimentological analyses reaching back the Late Pleistocene. High-resolution subaquatic imagery of the first tens of meters is required to understand Pleistocene/Holocene continental sedimentary basin infills. Sub-bottom profiler (SBP) technology is currently the best geophysical equipment to obtain the highest resolution imagery of underwater sediments. Resolution of such systems needs to be in the order of cm/dm to access centennial/millennial timescales. Continental scientific projects, however, suffer from a lack of portable & USV-designed SBP available on the market that can be easily operated in continental environments (lakes, river, lagoon, etc.).

In this context, Exail sonar system division, based in La Ciotat (France), has recently designed a new 10 kHz Chirp sub-bottom profiler for continental & shallow water investigations (5 – 15 kHz). Echoes Compact is a portable sub-bottom profiler for inland & coastal environments reaching in high-resolution Late Pleistocene & Holocene sedimentary archives. We focus our presentation on two case studies: one in maar lake Issarlès with paleosismological reconstructions in Massif central (Ardèche, France), and another in lagoon & coastal areas (Orbetello, Italy) throughout the recent publication from Brocard et al. (2024, Marine Geology), in which Echoes 10 kHz demonstrates outstanding performance in very shallow water environments (1m water depth/12 m penetration without multiple). We also present Echoes 3500 T1 geoscience applications, a 3.5 kHz system (1.8 – 6.2 kHz) with higher penetration & lower resolution than the Echoes Compact, with regards to its performance for exploring deeper coring sites especially in coarse sand environments.

Key words: sub-bottom profiler, acoustic, geophysics, geophysical software, shallow water

Brocard et al. (2024) Double tombolo formation by regressive barrier widening and landside submergence: The case of Orbetello, Italy. Marine Geology 477, 107415.

How to cite: Jouve, G., Chapron, E., and Gilles, B.: New Echoes Compact Sub-Bottom Profiler (SBP): Portable SBP for inland & coastal environments, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3145, https://doi.org/10.5194/egusphere-egu25-3145, 2025.

EGU25-3621 | ECS | Posters on site | GI1.1

Low-Frequency GPR as a Gateway to Archaeological Investigations: The Aeclanum’s Buried Roman-age Forum (Southern Italy) 

Nicola Angelo Famiglietti, Sandra Lo Pilato, Bruno Massa, Antonino Memmolo, Robert Migliazza, Massimo Osanna, Luana Toniolo, Antonietta Manco, and Annamaria Vicari

Ground Penetrating Radar (GPR) is a cornerstone technology in archaeological research due to its ability to non-invasively detect subsurface structures and artifacts. By emitting electromagnetic waves and analyzing their reflections, GPR enables researchers to map buried features with high precision while preserving the site's integrity. Low-frequency GPR systems, in particular, are well-suited for archaeological contexts, offering the depth penetration required to investigate complex stratigraphic settings and revealing structures that might otherwise remain undetected. The Archaeological Park of Aeclanum, located in Mirabella Eclano (AV), Southern Italy, is a site of great historical importance, hosting remains of a city that flourished under the Samnite and Roman civilizations. Among its most significant areas is the ancient Roman Forum, once the political, religious, and commercial heart of the city. Despite its historical relevance, the Forum had not yet been uncovered, and its exact layout and architectural features remained unknown. Previous investigations using higher-frequency GPR systems were limited in depth penetration, failing to detect deeper buried structures. To overcome these limitations, a low-frequency GPR survey was conducted in the Forum area. The survey employed a monostatic antenna with a center frequency of 80 MHz, enabling a maximum exploration depth of up to 5 meters, far exceeding the capabilities of previous investigations. This deeper penetration facilitated the identification of subsurface anomalies consistent with walls, pavements, and foundations. These anomalies provided the first geophysical evidence of the Forum’s layout and subsurface features, shedding light on a previously unexplored area. The GPR data revealed a series of significant anomalies, particularly at depths ranging from 1 to 3 meters. These features were interpreted as remnants of buried architectural elements associated with the Forum, including masonry walls, paved surfaces, and foundations. The ability to detect these features highlights the critical advantage of using low-frequency equipment in archaeological investigations. To validate the geophysical findings, targeted archaeological excavations were carried out in areas corresponding to the most prominent anomalies. These excavations uncovered well-preserved structural elements, including segments of masonry walls and paved surfaces, precisely matching the GPR-detected anomalies in location, depth, and geometry. Notably, the excavation confirmed the presence of foundational elements at greater depths, which were undetectable in previous surveys. The excellent spatial correlation between the GPR data and the exposed remains demonstrated the reliability and precision of the low-frequency GPR survey in reconstructing the Forum's layout. This study underscores the importance of selecting appropriate GPR configurations for specific archaeological objectives. By combining non-invasive geophysical techniques with targeted excavation, this integrated approach maximized the efficiency of the investigation while minimizing its impact on the site. The findings reinforce the potential of low-frequency GPR as a powerful tool in uncovering and preserving buried archaeological heritage.

How to cite: Famiglietti, N. A., Lo Pilato, S., Massa, B., Memmolo, A., Migliazza, R., Osanna, M., Toniolo, L., Manco, A., and Vicari, A.: Low-Frequency GPR as a Gateway to Archaeological Investigations: The Aeclanum’s Buried Roman-age Forum (Southern Italy), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3621, https://doi.org/10.5194/egusphere-egu25-3621, 2025.

EGU25-4149 | Orals | GI1.1

Shaping tomorrow's geospatial services: The DestinE Platform 

Alexis Longuet, Matteo Cortese, Calogera Tona, Daniele Pellegrino, Barbara Scarda, and Elisabetta Giuliani

The DestinE Platform represents the next generation of cloud-based geospatial services, enabling the integration and management of an ecosystem to facilitate the effective use and sharing of Earth Observation (EO) data. Designed as a distributed and federated digital ecosystem, the platform promotes seamless interaction among interconnected services, building on the concept of federations to support a diverse range of users: including both service providers and consumers such as citizens, researchers, businesses, and policymakers. This collaborative environment enables knowledge-sharing, cross-disciplinary analysis, and co-creation of geospatial solutions.

The platform provides a comprehensive suite of cloud-based services, including user management, Infrastructure-as-a-Service capabilities such as storage, networking, and CPU/GPU processing, data access and retrieval, data traceability and harmonisation, and 2D/3D visualisation tools. It also offers a core software suite for local data analysis, data and software cataloguing, and a flexible framework for service providers to host advanced DestinE applications. Through its use of OVHcloud-based infrastructure and federated services, including access to Copernicus data, the DestinE Platform empowers service providers to expand their offerings, increase visibility and drive innovation.

Cloud-based geospatial platforms are driving the evolution of Earth Observation (EO) services by adopting distributed infrastructures that integrate online data repositories, collaborative computing environments, and advanced data processing tools. The DestinE Platform facilitates the onboarding of external services and resources, fostering flexibility, scalability, and support for community-driven innovation. This approach unlocks new growth opportunities for service providers, offering greater visibility and pathways for and innovation, while emphasizing the importance of maintaining high-quality services to remain competitive.

By establishing clear conditions for participation, the DestinE Platform framework fosters equitable access to resources and strengthens engagement across its user community. This structured approach embodies the shift toward a federated digital ecosystem, capable of meeting the diverse requirements of modern geospatial data consumers and providers. By enabling interoperability and fostering shared development, the platform lays the groundwork for the next generation of Digital Earth ecosystems, shaping the future of EO technology and services.

How to cite: Longuet, A., Cortese, M., Tona, C., Pellegrino, D., Scarda, B., and Giuliani, E.: Shaping tomorrow's geospatial services: The DestinE Platform, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4149, https://doi.org/10.5194/egusphere-egu25-4149, 2025.

Accurate attitude determination is crucial for orbit determination and time-varying gravity field recovery in low-low Satellite-to-Satellite Tracking (ll-SST) missions, such as GRACE and its successor GRACE-FO. The acquisition of attitude information largely depends on the fusion of data from multiple star cameras (SCs) on board, where the covariance (i.e., noise) along each axis of each SC must be well known. Additionally, the covariance information is also vital for the subsequent reprocessing of the fused attitude. However, previous studies have assumed that the covariance is fixed and diagonal, which may not be realistic. Inspired by noise methods based on relative comparison analysis and combined with GNSS-based attitude determination performance research, considering GNSS-based attitude as an independent reference for spacecraft attitude helps quantify the SC's covariance matrix. Based on this, we propose a GNSS-aided Star Camera Fusion (GSCF) approach based on the quaternion-based generalized least squares principle for statistically optimal attitude determination in ll-SST missions. This method allows for the construction of dynamic noise models for attitude sensors and the acquisition of fused attitude covariance information, while also revealing the strong negative correlation between short-term covariance and solar angle during blind events, along with SC anomaly detection parameter. The study finds that, for daily GRACE-FO operations, compared to traditional methods, GSCF achieves an average improvement of 10 arcseconds in attitude determination, especially in the spectrum of the one Cycle -Per-Revolution (CPR) frequency and its harmonics. In terms of inter-satellite pointing variations, GSCF shows improvements in the pitch angle (maximum improvement of 1.1 arcseconds) and yaw angle (maximum improvement of 0.3 arcseconds). Additionally, GSCF has an impact on along-track measurements of up to 0.02 um/s. While these effects may be negligible for the current GRACE-FO mission, next-generation ll-SST gravity missions with ultra-high-precision payloads will be extremely sensitive to attitude determination, and the proposed GSCF method is expected to provide significant benefits in such missions.

How to cite: Pan, X., Yang, F., and Wu, Y.: A GNSS-aid star camera fusion approach towards statistically optimal attitude determination of ll-SST missions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5406, https://doi.org/10.5194/egusphere-egu25-5406, 2025.

EGU25-9794 | Orals | GI1.1

Soil H2 degassing studies: a useful geochemical tool for monitoring Cumbre Vieja volcano, La Palma, Canary Islands 

Eleazar Padrón, Jaia Kortman, Sophie Lyons-Montgomery, Oranna Reichrath, Ana Gironés, Daniela Taño, Laura Trujillo, Gladys V. Melián, María Asensio-Ramos, Nemesio M. Pérez, and Pedro A. Hernández

Hydrogen (H2) is one of the most abundant trace species in volcano-hydrothermal systems and is a key participant in many redox reactions occurring in the hydrothermal reservoir gas. Although H2 can be produced in soils by N2-fixing and fertilizing bacteria, soils are considered nowadays as sinks of molecular hydrogen. Because of its chemical and physical characteristics, H2 generated within the crust moves rapidly and escapes to the atmosphere.These characteristics make H2 one of the best geochemical indicators of magmatic and geothermal activity at depth. Regular surface geochemical studies have been conducted focusing on hydrogen (H2) emissions along Cumbre Vieja volcano (La Palma, Canary Islands) since 2001, encompassing the analysis of soil H2 content using a micro-gas chromatograph (Agilent 490 microGC) in samples collected at a depth of approximately 40 cm across 600 sites during each survey. Spatial distribution maps have been generated using sequential Gaussian simulation (sGs) techniques to quantify the diffuse H2 emissions from Cumbre Vieja volcano. The time series data of the diffuse H2 emissions indicate significant increases during the occurrence of seismic swarms observed between 2017 and 2021, reaching the maximum value of the series (36 kg·d-1) in June 2017, 4 month before the seismic swarms. During the eruptive phase, substantial spikes in the diffuse H2 emissions were observed, closely correlating with the volcanic tremor escalation. During 2024, the soil H2 emission ranged between 7 and 16 kg·d-1, values that can be considered within the background range. The absence of visible volcanic gas emissions before the eruption, such as fumaroles or hot springs, on the surface of Cumbre Vieja underscores the importance of such studies in serving as a critical tool for continuous volcanic surveillance and monitoring purposes. This update represents ongoing efforts to comprehensively study and understand the behavior of hydrogen emissions within the volcanic system, providing essential insights into volcanic activity and potential precursor signals for enhanced monitoring and risk assessment. 

How to cite: Padrón, E., Kortman, J., Lyons-Montgomery, S., Reichrath, O., Gironés, A., Taño, D., Trujillo, L., Melián, G. V., Asensio-Ramos, M., Pérez, N. M., and Hernández, P. A.: Soil H2 degassing studies: a useful geochemical tool for monitoring Cumbre Vieja volcano, La Palma, Canary Islands, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9794, https://doi.org/10.5194/egusphere-egu25-9794, 2025.

EGU25-10028 | ECS | Posters on site | GI1.1

Capabilities of LIMS in the Context of Trace Element Analysis and Provenance Determination of Gemstones 

Luca N. Knecht, Salome Gruchola, Peter Keresztes Schmidt, Marek Tulej, Andreas Riedo, and Peter Wurz

Colour variations within the same type of gemstone are caused by different abundances of trace elements. But apart from producing pretty colours, the analysis of the trace elements in gemstones is frequently used to distinguish between synthetic and natural specimen, for provenance determination, and treatment detection [1]. Every gemstone element composition is closely tied to its geological origin; thus, it is possible to determine the provenance according to those unique ‘fingerprints’. However, for some gemstones, such as sapphires, provenance determination remains challenging due to geologically similar deposits, consequently often leading to similar trace element abundances [2, 3].

This contribution presents the capabilities of a Laser Ablation and Ionization Mass Spectrometer (LIMS) instrument, called the Laser Mass Spectrometer – Gran Turismo (LMS-GT) [4, 5], in trace element analysis for gemstones. The study examined two samples (provided by the Swiss Gemmological Institute SSEF): a yellow sapphire, treated with beryllium diffusion to create the colour, and a synthetic dark blue spinel, produced via the Verneuil method. A gold coating was applied to mitigate surface charging effects, and peak-blanking was used to enhance the instrument’s limit of detection [6, 7].

The study focused on elements critical for provenance determination, including Mg, Ti, Fe, Ga, and other measured trace elements. The obtained data were compared to measurements performed with other instruments on the same gemstone varieties. This contribution will highlight the current progress of the study and discuss the advantages of the LMS-GT instrument in relation to other methodologies, emphasizing its potential to improve trace element detection and provenance determination in gemological research.

[1] S. Karampelas, et al., 2020, https://doi.org/10.1007/978-3-030-35449-7_3.

[2] Lee A. Groat, et al., 2019, http://dx.doi.org/10.5741/GEMS.55.4.512.

[3] M. Y. Krebs, et al., 2020, https://doi.org/10.3390/min10050447.

[4] M. Tulej, et al., 2021, https://doi.org/10.3390/app11062562.

[5] C. P. de Koning, et al., 2021, https://doi.org/10.1016/j.ijms.2021.116662.

[6] S. Gruchola, et al., 2022, https://doi.org/10.1016/j.ijms.2022.116803.

[7] S. Gruchola, et al., 2023, https://doi.org/10.1039/D3JA00078H.

How to cite: Knecht, L. N., Gruchola, S., Keresztes Schmidt, P., Tulej, M., Riedo, A., and Wurz, P.: Capabilities of LIMS in the Context of Trace Element Analysis and Provenance Determination of Gemstones, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10028, https://doi.org/10.5194/egusphere-egu25-10028, 2025.

EGU25-11125 | ECS | Posters on site | GI1.1

 The Current State of Active Time-Reverse Imaging: Defect Localization in Digital Concrete Physics 

Martin Balcewicz, Claudia Finger, Katrin Löer, and Erik H. Saenger

Ensuring the structural integrity of concrete, particularly in critical infrastructures like bridges, requires reliable methods for identifying and localizing small-scale defects, such as fractures or damage. This study introduces a non-destructive evaluation technique that leverages the principles of both active ultrasonic testing and passive seismic methods to enhance defect localization. The method, active time-reverse imaging (A-TRI), compares ultrasonic waveforms recorded from concrete specimens in their intact and altered states to pinpoint damage.

Unlike conventional time-reverse imaging approaches that primarily rely on passive signals, A-TRI utilizes an active ultrasound source to generate wavefields. These wavefields propagate through the medium, with multiple receivers capturing the resulting signals. The experimental workflow includes two main steps: (1) Ultrasonic waves are emitted into the concrete specimen from an active transducer while the signals are recorded by an array of receivers; (2) The experiment is repeated under identical conditions, but the concrete specimen includes a predefined defect in the case of one or more arbitrary localized inclusions. The differential signal—representing the changes introduced by the defect—is then reversed in time and used as the input for a subsequent simulation. This backpropagated wavefield converges at the location of the damage, effectively visualizing the defect.

The numerical experiments in this study utilize a heterogeneous concrete model with inclusions that mimic localized changes in material properties. We highlight the current limitations of the method, including scatter size and shape, the number of receivers, and signal length, among others. Imaging conditions are applied to evaluate the precision and success of defect localization.

The results demonstrate the capability of A-TRI to accurately identify and localize multiple defects, even in complex heterogeneous media. By combining active ultrasound methods with time-reverse principles, this approach offers a robust tool for the detailed assessment of concrete structures.

How to cite: Balcewicz, M., Finger, C., Löer, K., and Saenger, E. H.:  The Current State of Active Time-Reverse Imaging: Defect Localization in Digital Concrete Physics, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11125, https://doi.org/10.5194/egusphere-egu25-11125, 2025.

EGU25-11155 | Orals | GI1.1

Thermal Cone Penetration Test as a direct measurement of thermal conductivity of soils. 

John Paulo Idarraga Munoz and John Gregg

In situ measurement of the thermal conductivity of soils becomes relevant when laying structures which will dissipate heat. While the difference in thermal conductivity for different solids is relatively small compared to other physical properties, changes in porosity and soil consolidation will significantly change the effective thermal conductivity values. The goal is then not necessarily to perform a measurement with the objective of doing soil identification but as the means to understand the thermal conductivity properties locally, regardless of soil composition. Thermal data, along with industry standard measurements as described in ISO22476-1, can also be used to enhance the observable phase-space and thus improving discrimination capabilities. In this work, we introduce a new apparatus which can perform the in situ thermal conductivity measurement alongside industry-standard cone and piezocone penetration tests (CPTU) with unprecedented level of accuracy, while mitigating the impact of soil disturbances inherent to the cone penetration test.

How to cite: Idarraga Munoz, J. P. and Gregg, J.: Thermal Cone Penetration Test as a direct measurement of thermal conductivity of soils., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11155, https://doi.org/10.5194/egusphere-egu25-11155, 2025.

EGU25-12301 | Posters on site | GI1.1

G.O.Joe: A novel non-commercial software tool for the processing of LA-ICP-MS data 

Joachim Krause, Florian Altenberger, Thomas Auer, Alexander Auer, and Jasper Berndt

The coupling of laser ablation systems with inductively coupled plasma-mass spectrometers (LA-ICP-MS) was introduced in the 1980s. Since then, this technique has become indispensable for rapid, in-situ trace element and isotopic analysis of both natural and synthetic solid samples. Its applications extend across various fields, including chemistry, material science, geosciences as well as biological and environmental analysis, bio-imaging and forensic investigations. However, analytical advances are still needed to overcome problems in trace element analysis using LA-ICP-MS caused e.g. by interferences that cannot be solved instrumentally.

The novel and non-commercial software tool G.O.Joe is designed to facilitate the calculation of trace element mass fractions in solid samples obtained by LA-ICP-MS analysis. It is written in the Dart programming language using the Flutter framework and operates completely web-based, eliminating the need for installation and allowing access from any location with an internet connection. Since the calculation of the data itself is performed on the user’s computer, no upload of measured data to the G.O.Joe-server is necessary thereby maximizing data safety. In addition to a quick and efficient processing of large datasets (>400 analyses), G.O.Joe includes several types of optional interference corrections.

The intuitive user interface of G.O.Joe simplifies the workflow during data evaluation, including straightforward selections of peak- and background signals, importing instrument settings and reference material compositions as well as mass fractions of the internal standard to convert the measured raw signals into element mass fractions. To ensure a transparency in data processing, the results file (.xlsx) includes the calculated element mass fractions, associated statistical parameters as well as input data alongside instrument settings. In addition, the user can download a more comprehensive file with the results after each step of the calculation. The detailed Major advantages of the software are the implemented correction measures for isobaric interferences and abundance sensitivity.

G.O.Joe’s key features are presented by processing the mineral chemical analyses of two case studies, including trace element analyses of tungstates (e.g., scheelite) and silicates (e.g., garnet). Conclusively, G.O.Joe is a time-efficient, transparent and easy-to-use software, appealing to both experienced LA-ICP-MS users as well as newcomers to LA-ICP-MS data analysis. More details and the latest version of G.O.Joe are available at the following link: https://www.gojoe.software

How to cite: Krause, J., Altenberger, F., Auer, T., Auer, A., and Berndt, J.: G.O.Joe: A novel non-commercial software tool for the processing of LA-ICP-MS data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12301, https://doi.org/10.5194/egusphere-egu25-12301, 2025.

EGU25-17070 | Posters on site | GI1.1

Geographic authentication and quality assessment of Canary Islands Aloe: An isotopic and phytochemical approach 

Sttefany Cartaya-Arteaga, Mónica Arencibia, Ruth Rodríguez-Ramos, Beverley Claire-Coldwel, María Asensio-Ramos, Gladys V. Melián, Eleazar Padrón, Bárbara Socas-Rodríguez, Pedro A. Hernández, Miguel Ángel Rodríguez-Delgado, and Nemesio M. Pérez

The increasing European demand for high-quality, safe agricultural products have led to the development of stringent control measures to certify product authenticity and geographical origin, protecting both producers and consumers from potential fraud. This study focuses on Aloe Vera, a plant containing around 200 potentially active compounds of interest in the health and wellness industry, including vitamins, minerals, anthraquinones, and polysaccharides. The Canary Islands has a unique climate, which, combined with young volcanic soils, produce exceptionally high-quality Aloe Vera. However, fraudulent Aloe Vera products falsely labelled as having Canarian origin currently represent a 21 million euros market. This situation necessitates the development of reliable scientific protocols for geographical tracing of Canarian Aloe Vera and its derivatives (juices, gels, creams, cosmetics). Chemical profiling of Aloe Vera across the Canary Islands and the Iberian Peninsula includes the determination of strontium isotopic ratios (87Sr/86Sr) by thermal ionization mass spectrometry (TIMS) to trace geographic origin at certified grower plantations, complemented by phytochemical profiling to verify optimal growing conditions and quantitative quality standards. Complete Aloe Vera plants have been analysed, revealing distinct bioactive organic compounds of interest, including phenolic acids, flavonoids, terpenoids, anthraquinones and derivatives, among others. 87Sr/86Sr ratios in Canarian Aloe Vera plants are higher (0.7065-0.7078) than those expected from their dominantly basaltic volcanic soils (0.7032-0.7068), but lower than soil values observed in mainland Spain (0.7089-0.7124). Therefore, development of a full ´fingerprint´ profile of Canarian Aloe Vera must also quantify 87Sr/86Sr contributions from irrigation water sources and additives used in the growing and manufacturing process.

How to cite: Cartaya-Arteaga, S., Arencibia, M., Rodríguez-Ramos, R., Claire-Coldwel, B., Asensio-Ramos, M., Melián, G. V., Padrón, E., Socas-Rodríguez, B., Hernández, P. A., Rodríguez-Delgado, M. Á., and Pérez, N. M.: Geographic authentication and quality assessment of Canary Islands Aloe: An isotopic and phytochemical approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17070, https://doi.org/10.5194/egusphere-egu25-17070, 2025.

EGU25-17269 | Orals | GI1.1

Integrated geophysical studies at the OGS PITOP testing site: an interdisciplinary approach for subsurface characterization 

Andrea Travan, Cinzia Bellezza, Erika Barison, Piero Corubolo, Fabio Meneghini, and Andrea Schleifer

The OGS PITOP geophysical testing site, located in northeastern Italy, serves as a cutting-edge facility for developing and testing geophysical methods, technologies, and tools under realistic conditions. Covering an area of 22,000 m², PITOP is equipped with instrumented wells, permanent and mobile data acquisition systems, and active seismic and geoelectric sources. This infrastructure provides a unique environment for advancing subsurface characterization techniques.

The PITOP facility includes five wells (PITOP1-PITOP5) with depths ranging from 150 to 423 m. PITOP2 is equipped with 30 permanently installed three-axial geophones, while PITOP4 houses a Distributed Acoustic Sensing (DAS) fiber optic system. In March 2024, the addition of PITOP5 enabled a series of innovative experiments using the drill bit as a seismic source. These experiments had three primary objectives: (1) enhancing subsurface knowledge of the area, (2) testing new seismic instrumentation, and (3) performing integrated analyses using multidisciplinary methodologies.

During the PITOP5 drilling process, receivers were deployed both at the surface and in wells enabling cross-well tests acquired while drilling. The Seismic While Drilling (SWD) technique utilizes the drill bit as the seismic source. Surface receivers included standard geophones and triaxial nodes, arranged symmetrically around PITOP5.

In addition to SWD, Vibroseis was employed as an active seismic source, complementing the drill bit experiments. This enabled a comparison of results from different seismic energization methods, further enhancing the robustness of the dataset.

Preliminary seismic data analysis revealed the presence of shallow/medium depth reflectors.

Complementary to the seismic investigations, the PITOP5 upgrade included geoelectrical instrumentation. An array of electrodes was installed and cemented within the PITOP5 well to a depth of 260 m, allowing for advanced geoelectrical analyses and interdisciplinary investigations of the subsurface including the seismic methods.

Overall, a key feature of the PITOP upgrade is its capability for integrated geophysical experiments. During the drilling of PITOP5, surface seismic, SWD, and cross-hole experiments were conducted using diverse sources and acquisition systems. Data processing and integration are ongoing, with the aim of combining seismic and electrical information to provide a comprehensive understanding of subsurface structures.

The PITOP testing site represents a significant advancement for the scientific and technical community, offering a versatile platform for multidisciplinary studies. Its capabilities are particularly relevant for projects related to CO2 and energy storage, both of which are critical for climate change mitigation and the transition to sustainable energy systems.

With its state-of-the-art infrastructure and recent upgrades, PITOP is positioned as a leading facility for applied geophysics. The site not only facilitates the development of innovative geophysical techniques but also fosters collaboration among researchers, paving the way for future advancements in geosciences.

References

Geophysical exploration case histories at the geophysical test site PITOP - a key facility in the ECCSEL-ERIC consortium: an overview. Bellezza et al., Bulletin of Geophysics and Oceanography, 2025

How to cite: Travan, A., Bellezza, C., Barison, E., Corubolo, P., Meneghini, F., and Schleifer, A.: Integrated geophysical studies at the OGS PITOP testing site: an interdisciplinary approach for subsurface characterization, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17269, https://doi.org/10.5194/egusphere-egu25-17269, 2025.

EGU25-17365 | Posters on site | GI1.1

Soil CO2 efflux and hydrogeochemical monitoring for volcanic surveillance of Tenerife, Canary Islands, Spain 

Mónica Arencibia Hernández, Jorge Hernandez Fung, Sttefany Cartaya, Gladys V. Melián, María Asensio-Ramos, Eleazar Padrón, Nemesio M. Pérez, Pedro A. Hernández, and Germán D. Padilla

Tenerife island, with 2034 km2, is the largest active volcanic island of the Canarian archipelago and has remained in a state of volcanic calm since the Chinyero eruption in 1909. Apart from the fumarolic activity present at the summit crater of Teide volcano, nowadays not any visible evidence of gas emission is found at Tenerife. The main geophysical event recorded in Tenerife in the study period is a significant seismic swarm of long-period events recorded on 2 October 2016, with a subsequent significant increase in seismic activity recorded in and around the island observed to date. As part of the INVOLCAN Volcano monitoring program for the reduction of volcanic risk in Tenerife and with the aim of strengthening the geochemical monitoring program, we have conducted on a weekly basis, two distinct studies: (1) physical-chemical and chemical/isotopic composition studies in the groundwater of two galleries (Fuente del Valle and San Fernando) and its associated dissolved gases from mid-2016 to the present; and (2) a weekly study (since March 2024) of diffuse CO2 emissions at 31 selected points along the three volcanic-ridges of the island (NE, NW, and NS)  and Las Cañadas caldera (central volcanic complex). 

The most relevant results obtained in the hydrogeological study, were significant changes observed during and after the 2 October 2016 seismic swarm measured in the dissolved gases (CO2 and He), likely produced by the dissolution of volcanic hydrothermal gases released after the input of magmatic fluids in the groundwater system. This study underscores the sensitivity of monitoring the chemical and isotopic composition of groundwater in Fuente del Valle and San Fernando galleries to fluctuations in volcanic activity on Tenerife.  

The diffuse CO2 emissions values measured at the 31 selected points ranged between non-detected values (<0.5 g·m-2d-1) and 26.2 g·m-2d-1, with maximum values measured in Las Cañadas caldera and the north-east volcanic ridge. Although the values ​​recorded have been low, with values ​​typical of biogenic degassing, the time series that began in March 2024 serves as a baseline in periods of volcanic calm to assess possible future increases related to changes in the activity activity of Tenerife.

How to cite: Arencibia Hernández, M., Hernandez Fung, J., Cartaya, S., Melián, G. V., Asensio-Ramos, M., Padrón, E., Pérez, N. M., Hernández, P. A., and Padilla, G. D.: Soil CO2 efflux and hydrogeochemical monitoring for volcanic surveillance of Tenerife, Canary Islands, Spain, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17365, https://doi.org/10.5194/egusphere-egu25-17365, 2025.

EGU25-18834 | Posters on site | GI1.1

Revealing the hidden seismicity of Tenerife (Canary Islands) through machine learning and cross-correlation 

Luca D'Auria, Lucía Mesa Jiménez, Ismael Santos Campos, Aarón Álvarez Hernández, Rubén García Hernández, David Martínez van Dorth, Víctor Ortega Ramos, Germán D. Padilla Hernández, and Nemesio M. Pérez Rodríguez

In recent years, the development of techniques based on integrated machine learning techniques with traditional methods like cross-correlation has dramatically improved the capability of detection, location and characterisation of seismic events.

Machine learning-based techniques have been applied to improve earthquake catalogues, aiding seismicity analysis in different geodynamic contexts. These techniques are especially valuable in volcanic and geothermal contexts, where volcano-tectonic earthquakes and long-period events have low magnitude, often preventing a successful manual analysis. Since 2016, the island of Tenerife has been affected by increased seismicity and gas emissions from the crater of Teide volcano, the most prominent feature of the island of Tenerife. We applied the software Qseek (https://github.com/pyrocko/qseek) to enhance the seismic catalogue based on manual detections in Tenerife.

This reanalysis of Tenerife's seismic dataset revealed intense seismicity related to episodes of magmatic fluid injection into the upper crust. Subsequently, high-resolution relocation techniques based on the software GrowClust (https://github.com/dttrugman/GrowClust) imaged the spatial pattern of the hypocenters, highlighting sources of magmatic fluid injection into the hydrothermal system of Tenerife and the subsequent response of the upper crust to this disturbance.

How to cite: D'Auria, L., Mesa Jiménez, L., Santos Campos, I., Álvarez Hernández, A., García Hernández, R., Martínez van Dorth, D., Ortega Ramos, V., Padilla Hernández, G. D., and Pérez Rodríguez, N. M.: Revealing the hidden seismicity of Tenerife (Canary Islands) through machine learning and cross-correlation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18834, https://doi.org/10.5194/egusphere-egu25-18834, 2025.

EGU25-20014 | Orals | GI1.1

DTEClimate: A Digital Platform for Real-Time Geospatial Intelligence and Climate Monitoring 

Angela Constantin, Adrian-Iulian Brezulianu, Mihaela Gavrila, Delia-Elena Barbuta, Constantin Ionescu, and Victorin Toader

Geospatial intelligence involves the analysis and interpretation of spatial data to inform decision-making. Understanding and responding to geospatial phenomena, such as seismic events or atmospheric disturbances, is essential for advancing disaster preparedness and environmental monitoring. However, significant challenges arise from the lack of integrated systems capable of securely collecting, processing, and analyzing large-scale geoscience data.
To address this, the "Digital Twin Earth Intelligence for Climate Changes" (DTEClimate) project has developed a platform that integrates real-time data gathered from various sensors, to create visual maps, easily accessible for the general public. In order to process all this data, integration services have been developed, which continuously monitor and process data gathered by sensors. This stored data is then used to create multi-layered maps representing various event types and heatmaps illustrating data concentrations.
On the one hand, in our platform users can visualize the progression and current status of meteorological events, which improves awareness. On the other hand, researchers can use the aggregated data to better monitor the environment or conduct multidisciplinary analyses to explore the interdependencies among different environmental parameters. By bridging the gap between real-time data collection and data visualization, DTEClimate aims to empower both the public and scientific communities to make data-driven decisions in the face of climate change and natural disasters.

Acknowledgements

This work was carried out within PNRR-DTEClimate/REACTIVE project, no. 760008/30.12.2022.

How to cite: Constantin, A., Brezulianu, A.-I., Gavrila, M., Barbuta, D.-E., Ionescu, C., and Toader, V.: DTEClimate: A Digital Platform for Real-Time Geospatial Intelligence and Climate Monitoring, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20014, https://doi.org/10.5194/egusphere-egu25-20014, 2025.

EGU25-20391 | Orals | GI1.1

Potential of on-board FTIR as a single instrument for simultaneous measurement of all gaseous pollutants of interest under real-driving conditions. 

Hannu Kuutti, Michal Vojtisek, Michal Vojtisek, Lubos Dittrich, Lubos Dittrich, and Martin Pechout

Responding to the outdoor air pollution being one of the gravest environmental hazards to human health, emissions from mobile sources have been subject to scrutiny and emissions reduction efforts through improved fuels, engine design, combustion control, exhaust aftertreatment, and traffic management. Assessment of the effects of various improvements has gradually extended from basic laboratory measurements to testing under real-world (real-driving) conditions and to additional pollutants.

Fourier-transform infra-red (FTIR) spectrometers have the potential to acquire spectra at high optical and time resolution. The absorption spectra are a convolution of absorption spectra of individual compounds and can be, with varying success, interpreted to obtain the concentrations of the pollutants of interest. To date, several FTIR have been adopted for the use in moving vehicles, which is challenging due to the effects of vibrations on precision multipath low-volume optical cells used to achieve a fast response time. The validation of on-road FTIR instruments typically consists of parallel measurement with reference instruments in the laboratory for all measured pollutants and on the road for those pollutants that can be reliably measured on the road.

In this work, two FTIR analyzers adapted for on-road use, an A&D BOB-1000FT vacuum sampling system operating at 5 Hz and a 35-kg Bruker Matrix extensively modified by Czech University of Life Sciences operating at 2.5 Hz, both with a 5-meter multipath cell and 0.5 cm-1 optical resolution, were used to sample the exhaust from diesel, gasoline and natural gas vehicles with and without exhaust aftertreatment. Concentrations and emissions of all pollutants set to be regulated under Euro 7, health and environment relevant reactive species reactive nitrogen species NO, NO2, NH3, CO and formaldehyde, and greenhouse gases CO2, CH4 and N2O were measured during dynamic driving cycles at -9 C, +23 C and + 35 C ambient temperatures.

The results show a reasonable correlation with reference instruments for all evaluated pollutants, suggesting on-board FTIR, which is not much larger than other instruments used to measure real driving emissions, can be potentially used to measure all gaseous pollutants regulated under Euro VII/7 on the road. FTIR spectra can be, even ex-post, interpreted for additional pollutants of interest.

 

Funding: This work was supported by the European Union’s Horizon Europe research and innovation programme under grant agreements No 101096133 (PAREMPI: Particle emission prevention and impact: from real world emissions of traffic to secondary PM of urban air) – experiments and No. 101056777 (LENS, L-vehicles Emissions and Noise Mitigation Solutions) – FTIR development.

How to cite: Kuutti, H., Vojtisek, M., Vojtisek, M., Dittrich, L., Dittrich, L., and Pechout, M.: Potential of on-board FTIR as a single instrument for simultaneous measurement of all gaseous pollutants of interest under real-driving conditions., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20391, https://doi.org/10.5194/egusphere-egu25-20391, 2025.

EGU25-2316 | Posters on site | GI1.3

Development of an intelligent recirculating water system for land-based sea cucumber aquaculture 

Kuo-Hua Chien, Wen-Shun Huang, Jinn-Chyi     Chen , and Xiangfei   Ren 

  Presently, three fundamental methods are employed for sea cucumber aquaculture: pond culture, dam culture, and submarine seedling culture. However, these methods are susceptible to environmental water quality degradation due to factors such as sea cucumber feces, excessive feed, and climate change, which can impede sea cucumber growth and affect yields.

In order to address the issues outlined above, this study presents the intelligent circulating water system (ICWS), which is composed of a composite low-energy physical liquid-solid separator and a multi-mixed biofilter. A detailed description of these components is provided below.

  • Composite Low Energy Physical Liquid-Solid Separator

The liquid-solid separator uses minimal energy because of its innovative composite type. It extracts the contaminant source from the aquatic environment, reducing biofilter bed load and energy demand.

  • Multi-mixed Biofilter

The configuration of hybrid arrangement structures increases the specific surface area of the biofilter, leading to a reduction in its volume. The structure controls flow rate, hydraulic residence time, and hydraulic loading, which can be used to regulate temperature, salinity, pH, dissolved oxygen, and ammonia levels. This ensures the provision of high-quality water that meets the needs of sea cucumbers.

The innovative low-energy-consuming water recycling system outlined in this project has the theoretical potential to achieve complete water recycling without the necessity of replenishing the source water. This scenario presents a mutually beneficial opportunity for the sustainable utilization of Earth's water resources and the realm of commercial aquaculture, exhibiting no inherent incompatibility.

How to cite: Chien, K.-H., Huang, W.-S., Chen , J.-C.  .  ., and Ren , X.  .: Development of an intelligent recirculating water system for land-based sea cucumber aquaculture, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2316, https://doi.org/10.5194/egusphere-egu25-2316, 2025.

EGU25-4974 | ECS | Posters on site | GI1.3

Improving Discharge Measurement in Unmeasured Zones of ADCPs 

Jongmin Kim and Dongsu Kim

The Acoustic Doppler Current Profiler (ADCP) is one of the most commonly used instruments for measuring river discharge by utilizing the Doppler effect of acoustic waves. However, its reliance on a single transducer introduces certain limitations. During the transition between transmission and reception of the acoustic signal, the returning signal cannot be captured, resulting in an inability to measure discharge near the sensor.

Additionally, side-lobe interference generated by acoustic waves reflects off the riverbed and contaminates measurements near the bottom. To mitigate this, discharge data within 5% of the water depth from the bottom are typically excluded from results. Furthermore, in shallow areas where the unmeasured regions near the sensor and near the bottom overlap, discharge cannot be accurately measured.

To address these gaps, discharge in the unmeasured regions of ADCP measurements is typically extrapolated using data from the measured sections or calculated using empirical equations. In this study, a method to improve the measurement accuracy in the unmeasured regions of the ADCP was developed and evaluated.

 

Acknowledgements 

This work was supported by Korea Environment Industry & Technology Institute(KEITI) through Research and development on the technology for securing the water resouces stability in response to future change Program, funded by Korea Ministry of Environment(MOE)(RS-2024-00336020)

How to cite: Kim, J. and Kim, D.: Improving Discharge Measurement in Unmeasured Zones of ADCPs, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4974, https://doi.org/10.5194/egusphere-egu25-4974, 2025.

EGU25-9193 | Posters on site | GI1.3

Monitoring for  sustainable and inclusive urban areas 

Francesco Soldovieri, Vincenzo Cuomo, and Jean Dumoulin

Urban areas need to rethink their policies to strengthen their capacities to prepare for and respond to hazards and become more resilient, intelligent and inclusive. In this context, one of the objectives is to ensure the resilience of their services and systems against multi-hazard scenarios, where the effect of local hazards combines with global challenges such as climate change and pandemics. Moreover, the concept of inclusiveness is becoming crucial, as highlighted during COVID, which showed that the most vulnerable population is the one living in sparsely and densely populated areas, where the level of social and physical services is often inadequate [1].

In this context, one possible response to this need is the development of monitoring and surveillance approaches [2]. The present contribution will focus on three aspects

The first is that resilience must be addressed as a whole, since services and networks are interconnected and interdependent (e.g. health system, transport, energy and water distribution, air quality, protection from extreme weather events, etc.). The main consequence of these interconnections is that the complete collapse of services (blackout) may become a realistic possibility.

The second aspect is that resilience can only be achieved in the presence of continuous and detailed monitoring of both the structures/infrastructure/services and the territory on which they insist, and that without such a monitoring it is impossible to correctly define the interventions to be carried out and their priorization.

The third aspect concerns the development of new monitoring systems based on Earth observation, positioning, navigation, and ICT technologies that exploit the citizen as a sensor and the so-called ‘non-sensors’, i.e. sensors that provide useful information for monitoring even if they are not designed for this purpose. All this ‘sensory’ data must be integrated to obtain a complete and reliable awareness of the scenario; hence the need to process and systematize large amounts of information that can only be processed by AI and HPC.

 

[1] V. Cuomo F. Soldovieri F. Bourquin, N. -E. El Faouzi, J. Dumoulin. The necessities and the perspectives of the monitoring/surveillance systems for multi-risk scenarios of urban areas including COVID-19 pandemic. Proceedings of the TIEMS Annual Conference, 18-20 November 2020, Paris, France, ISBN: 978-94-90297-19-0, vol. 27

[2] Cuomo V., Soldovieri F., Ponzo F.C., Ditommaso R. (2018). A holistic approach to long-term SHM of transport infrastructures. The International Emergency Management Society (TIEMS) Newsletter 33, pp. 67-84.

How to cite: Soldovieri, F., Cuomo, V., and Dumoulin, J.: Monitoring for  sustainable and inclusive urban areas, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9193, https://doi.org/10.5194/egusphere-egu25-9193, 2025.

EGU25-10582 | Orals | GI1.3

Near real-time, water quality event monitoring in small rivers, in the context of increasing frequency and intensity of hydrodynamic events due to climate change. 

Lisa Cronin, Cian M. Taylor, Ciprian Briciu-Burghina, Fiona Regan, and Frances E. Lucy

Freshwater quality continues to decline despite the adoption of the Water Framework Directive (WFD) almost twenty five years ago with the recovery of water quality in Europe plateauing since the 2010s (Haase et al., 2010).  Pollution from diffuse sources, particularly from agriculture remains a key challenge to restoring water quality to at least ‘good status’ under the WFD (EEA, 2018) compounded by water quality declines due to increased frequency and intensity of hydrodynamic events (van Vliet et al., 2023). 

Assigning accurate WFD classes and detecting changing trends in water quality have been challenging where traditional low frequency monitoring approaches have been implemented (Skeffington et al., 2015).  Higher monitoring frequency and spatial coverage is required to effectively identify improvements in water quality (Westerhoff et al., 2022) particularly when detecting changes over shorter time periods (Mcdowell et al., 2012).  High frequency monitoring is required to identify temporal water quality changes linked to rainfall driven pollutant transfer from land to waters (Métadier and Bertrand-Krajewski, 2012) with monitoring over multiple events required to capture the variability in pollutant concentrations and pollutant loads across events (Kozak et al., 2019).  Furthermore, 50% of surface waterbodies in the EU are impacted by multiple pressures (EEA, 2018), with increased urbanisation requiring a more complex, multi-pollutant approach to assessing impacts on river quality (Strokal et al., 2021).

The aim of this research was to identify if rainfall driven transient pollution events were occurring at two monitoring stations in a river catchment, and if continuous instream monitoring of turbidity and other water quality parameters could be used to capture changes in water quality and potential instances of such events.  One of the objectives was to identify if continuous monitoring could create a site-specific water quality profile that could be used to identify early warning indicators of rainfall driven or other transient pollution events. 

Results from this study indicate that changes in water quality are happening during rainfall events and that turbidity alongside other parameters can be used to track such events, trigger alarms when a probable event is occurring and automatically activate more intense monitoring during these events.  The integrated monitoring approach adopted allows for the tracking of water quality changes across temporal and spatial scales for multiple pollutants and allows for temporal fluctuations, and variation in pollutant loads during hydrodynamic events to be determined. 

The significant advantages of this approach are it’s suitability for remote deployments with no requirement for permanent infrastructure, the use of site specific water quality profiles to identify potential water quality events at individual sites and to activate further monitoring if required, the ability to tailor the monitoring for pollutant screening or more specific pollutants of concern, and the cost effectiveness of moving the integrated monitoring station between different water bodies. 

How to cite: Cronin, L., Taylor, C. M., Briciu-Burghina, C., Regan, F., and Lucy, F. E.: Near real-time, water quality event monitoring in small rivers, in the context of increasing frequency and intensity of hydrodynamic events due to climate change., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10582, https://doi.org/10.5194/egusphere-egu25-10582, 2025.

EGU25-10725 | ECS | Posters on site | GI1.3

Advanced Ultrasound Techniques for Investigating Air-Water Two-Phase Flow: An Experimental Approach 

Juan Calderon, Max Dormann, Till Branß, Martin Balcewicz, Jochen Aberle, and Erik Saenger

The König-Project, funded by the German state, is a long-term project focused primarily on developing a multi-scale wave measurement laboratory to improve flow measurements in an industrial context. Part of this project researches the propagation of ultrasound waves inside a moving fluid. A wide variety of flow scenarios are considered, and new methods for ultrasonic flow measurement can be developed and optimized. One experimental scenario includes the determination of volume fraction and drop size distributions of air dispersed in water using ultrasonic waves.

For this purpose, a modular system is used as an initiative to integrate manufacturer-independent measurement components with open-source software for the acquisition and processing of ultrasound signals. The modular system equipment consists of a multichannel system, which allows the positioning of several transceivers to send and receive ultrasonic waves from different directions along the experimental zone of interest. The concentration of dispersed air in water will be determined by measuring the reduced transit time caused by the added compressibility of the air phase.

Characterizing multiphase flows using other techniques can be time-consuming and the accuracy can fall short as the complexity of the fluid grows. The use of ultrasound to characterize fluid flows has many advantages such: as a non-invasive method that doesn’t alter the fluid path, real-time data acquisition, and high-temporal resolution, it is cost-effective and can be used on opaque fluids. Therefore this technique is gaining more attention in several industrial applications, including oil and gas, hydrogen, and geothermal energy generation. The results of this investigation will be validated and compared with the output of a numerical simulation, in which the boundary conditions and the flow characteristics will be similar to the experimental setup.

 

How to cite: Calderon, J., Dormann, M., Branß, T., Balcewicz, M., Aberle, J., and Saenger, E.: Advanced Ultrasound Techniques for Investigating Air-Water Two-Phase Flow: An Experimental Approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10725, https://doi.org/10.5194/egusphere-egu25-10725, 2025.

EGU25-10832 | ECS | Posters on site | GI1.3

Numerical Study to Determine Water-Air Dispersion with Ultrasound Waves 

Max Dormann, Juan Calderon, Claudia Finger, Martin Balcewicz, and Erik H. Saenger

The König-project is funded by the German state with the aim to develop a calibrated and virtual measurement laboratory to enhance methods based on ultrasound measurements that find application in the determination of flow velocity or particle movement. By comparing the results of controlled laboratory and real-world experiments with numerical simulations, the understanding of the interaction between ultrasonic waves and fluid flow is intended to be improved. The amount of scatterers within a fractured medium directly affects  the effective velocity of elastic waves. Thus we investigate, if the effects found in solid media can be transferred to fluids. We ran a series of numerical experiments, simulating ultrasound transmission measurements for multiple concentrations of bubbles of varying diameter dissolved in a stationary water layer. For the simulation of elastic wave propagation, we used a rotated staggered finite-difference scheme. We investigate the relation between the effective wave speed and the bubble concentration and compare those to results of laboratory experiments. Future research will then expand to moving fluid-gas mixtures.

How to cite: Dormann, M., Calderon, J., Finger, C., Balcewicz, M., and Saenger, E. H.: Numerical Study to Determine Water-Air Dispersion with Ultrasound Waves, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10832, https://doi.org/10.5194/egusphere-egu25-10832, 2025.

EGU25-10867 | Posters on site | GI1.3

Radar Altimetry Reveals the Smoothness of the Surface: the Case of Salar de Uyuni, Bolivia 

Francesco De Biasio, Stefano Vignudelli, Ron Abileah, and Paula Pacheco Mollinedo

Salar de Uyuni is a salt desert in Bolivia, spanning approximately 10,000 km2. During the wet season a thin layer of rainfall water covers the salt flats, making its surface mirror-like and earning it the title of “the largest natural mirror in the world”. The surface reflects the sky like a mirror, and attracts tourists who document this effect only from its outer perimeter. No evidence is documented in the interior, accessible only during the dry season. The only frequent observations of the Salar surface are from satellites, particularly altimetric radars, which are specifically designed to measure topography. Originally developed to measure sea level [1], they have recently been used, with a different metrics, to describe how emitted radar pulses are reflected by the surface, measuring the intensity of the reflected echo, and thus the Radar Cross Section (RCS) of the surface [2]: higher RCSs correspond to smoother surfaces. RCS was initially estimated in [1] with a an approximate method. Later EUMETSAT shared a better estimate by solving the radar equation with satellite parameters that were previously unknown to us [3]. In this study we used Sentinel-3A and 3B RCS measurements over the Salar flats, along six ground tracks, to describe for the first time the evolution of the Salar surface smoothness in space and time. A field campaign (16th - 20th of February 2024) was also conducted to validate the interpretation of radar measurements during the Sentinel-3A overpass on the track 167. At the field site, in a water depth of 1.8 cm (horizontal wind 4.5-3.4 ms-1), we measured a null vertical surface displacement to within ±0.5 mm, which classifies the surface as electromagnetically smooth at the radar frequency. The RCS values near the site were around 120 dBsm, as expected for radar return from a smooth surface. Three peaks are observed on the statistical distribution of the RCS: 87 (dry), 101 (intermediate) and 120 dBsm (wet season).The wet season, characterized by values above 101 dBsm, begins in December, peaking from late January to early March. February thus ensures the highest chance to observe mirror-like effects. Rainfall climatology from Uyuni city meteorological station reflects such statistics. The spatial and temporal evolution of RCS over the Salar, however, do not describe this place like a uniform mirror at the radar frequency, and so it is unlikely to observe such effect at shorter wavelengths, contrary to what is believed in the literature. Finally, satellites can help tourism stakeholders in programming the most enjoyable experience for travellers.

[1] Vignudelli et all. 10.1007/s10712-019-09569-1

[2] Abileah and Vignudelli, 10.1016/J.Rse.2021.112580

[3] Dinardo and Lucas, EUM/RSP/TEN/23/1376566

How to cite: De Biasio, F., Vignudelli, S., Abileah, R., and Pacheco Mollinedo, P.: Radar Altimetry Reveals the Smoothness of the Surface: the Case of Salar de Uyuni, Bolivia, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10867, https://doi.org/10.5194/egusphere-egu25-10867, 2025.

EGU25-12996 | Orals | GI1.3

Integrating Remote Sensing Technique with 3D Numerical Modelling for Enhanced Maintenance of Critical Infrastructure in Landslide-Prone Areas 

Diana Salciarini, Alice Vitaletti, Erica Cernuto, and Filippo Ubertini

Landslides, alongside earthquakes and floods, are among primary natural phenomena that are responsible for significant social and economic losses. Their impact poses an increasing threat worldwide, particularly in marginal and degraded contexts, affecting urban areas, infrastructures, environmental, historical, and cultural heritage, and, in severe cases, resulting in human casualties. In recent years, the number of infrastructure collapses or severe structural damages due to landslide movements has risen significantly, hindering the functionality of infrastructures, and highlighting the urgent need to deeply understand their interactions. Landslides can endanger roads, bridges, and railways, compromising the accessibility and inclusivity, and exacerbating social and economic exclusion in affected areas. Critical infrastructures are often located in challenging areas, where the susceptibility to landslides and natural hazards is significantly elevated. These sites demand advanced monitoring technologies to ensure infrastructure safety and mitigate the social and economic impacts of landslides. This study explores an innovative approach that integrates Interferometric Synthetic Aperture Radar (InSAR) data with numerical Finite Element Modelling (FEM) to address these challenges. The proposed method was applied to a case study involving a partial interaction between a slow-kinematic landslide, documented in the Inventory of Landslide Phenomena in Italy (IFFI), and a bridge along a highway section in the Liguria Region. Leveraging high-resolution satellite-based data from the Copernicus European Ground Motion Service (EGMS), the InSAR analysis provided spatial and temporal monitoring of ground displacements. Satellite remote sensing offers a wide spatial and temporal coverage over multiple regions, enabling for the detection of extensive or hard-to-access areas with millimetric precision in deformation velocity, ensuring high efficiency at a favourable cost-benefit ratio. However, while InSAR analysis can precisely measure ground motions, it lacks the ability to provide insights into the physical mechanisms under varying loading conditions. To address this limitation, FEM modelling was used to simulate the three-dimensional landslide mechanical behaviour under hydraulic loading, offering a deeper understanding of the slope stability and infrastructure deformations. InSAR data post-processing enabled the estimation of transverse and vertical components of the actual displacement vector, aligning with the observed landslide deformations and facilitating the numerical model validation. Simultaneously, FEM results highlighted significant displacements downstream of the landslide area, indicating a slope stability close to the limit equilibrium condition. Quantitative analysis also revealed relevant deformations at the base of bridge piers located within the landslide, caused by horizontal forces impacting the foundations. The integration of InSAR observations and FEM calculations demonstrated consistency in the identified movement, validating the efficacy of the combined method in identifying critical zones in landslide-prone regions. This study highlights how advanced remote sensing technologies, when coupled with numerical simulations, can enhance the monitoring and maintenance of critical infrastructure, particularly in marginal or extensive contexts. By identifying vulnerable areas and supporting the maintenance strategies, this methodology can contribute to hydrogeological risk management and promote inclusivity in regions where social and economic disparities exacerbate natural hazards impacts.

How to cite: Salciarini, D., Vitaletti, A., Cernuto, E., and Ubertini, F.: Integrating Remote Sensing Technique with 3D Numerical Modelling for Enhanced Maintenance of Critical Infrastructure in Landslide-Prone Areas, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12996, https://doi.org/10.5194/egusphere-egu25-12996, 2025.

EGU25-13576 | Orals | GI1.3

An Approach for IoT-Based Smart Sensors Placement in Urban Water Networks Under Natural Hazards 

Bahram Malekmohammadi, Mehdi Rahimi, Reza Kerachian, Vijay P. Singh, Roger A. Falconer, Roohollah Noori, and Farhad Bahmanpouri

Natural hazards such as floods, storms, and earthquakes present significant threats to urban infrastructures, particularly water supply and distribution networks. These events can severely impact the quality and quantity of water resources, leading to serious consequences for public health and social security. Factors such as unplanned urban development and non-compliance with engineering standards further increase the vulnerability of these systems. Recent advancements in technologies like the Internet of Things (IoT) and Artificial Intelligence (AI) have enabled real-time monitoring and data analysis of these critical infrastructures. IoT-based smart sensors capture essential information, including flow rate, water quality, corrosion, leakage, and pipeline ruptures. These data are processed using machine learning and deep learning algorithms to identify anomalies. Such systems can enhance monitoring capabilities and support effective decision-making in crisis situations. This study explores key criteria for selecting optimal locations for sensor deployment. These criteria include connection points, infrastructure accessibility, water quality, natural hazard risks, and historical incident data. For example, evaluating the location of connection points and their impact on water flow and distribution can help identify optimal routes, reducing costs and response times. Easy access to infrastructure facilitates sensor installation and maintenance, improving system efficiency. Monitoring water quality at various points in the distribution network is also critical to identifying sensitive locations and ensuring water safety. Additionally, identifying areas prone to natural hazards helps prioritize vulnerable regions for monitoring and improve system resilience. Historical data on anomalies and past incidents provide patterns that highlight risk-prone areas and help refine monitoring strategies. Based on these criteria, a multi-criteria decision-making approach is applied to propose the most effective locations for sensor placement. This method suggests prioritizing locations that have the highest impact and accessibility. These recommendations aim to enhance system efficiency and improve response capabilities during emergencies.

Ketwords: Smart Infrastructures, Internet of Things, MCDM, Artificial Intelligence, Natural Hazards

How to cite: Malekmohammadi, B., Rahimi, M., Kerachian, R., Singh, V. P., Falconer, R. A., Noori, R., and Bahmanpouri, F.: An Approach for IoT-Based Smart Sensors Placement in Urban Water Networks Under Natural Hazards, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13576, https://doi.org/10.5194/egusphere-egu25-13576, 2025.

EGU25-17346 | Orals | GI1.3

Drone based radar technologies for wide rural areas resources exploration: potentialities and challenges 

Ilaria Catapano, Giuseppe Esposito, Gianluca Gennarelli, and Francesco Soldovieri

Rural areas, i.e. areas with a low population density and a small number of anthropogenic environments, represent a significant resource in the pursuit of a green and sustainable development of the European Community [1]. This development involves not only the ecological and balanced use of agriculture and forestry resources, but also policies devoted to environmental protection and monitoring. In this context, drone-based technologies offer valuable opportunities because they facilitate the effective and non-invasive surveillance and monitoring of wide and inaccessible places. These technologies, indeed, allow surface and subsurface explorations, while concomitantly reducing the financial and logistical demands associated with investigation missions.

The present contribution is focused on Unmanned Aerial Vehicle (UAV)-Ground Penetrating Radar (GPR) technology and the potential of UAV-GPR technological solutions in subsurface prospecting [2]. The discussion encompasses the collection and processing of data, emphasising the efficacy and sustainability of the technology. The contribution will address the development of guidelines for the design of the flight grid and the formulation of an effective imaging strategy that can account for deviations in motion relative to the nominal trajectory.

[1] Bizottság, E. (2024). The long-term vision for the EU’s rural areas: key achievements and ways forward. Report from the Commission to the European Parliament, the Council, the European Economic and Social Committee and the Committee of the Regions, Brüsszel, The long-term vision for the EU’s rural areas: key achievements and ways forward, Report from the Commission [Letöltve: 2024.06. 20.].

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

Acknowledgements: The communication has been funded by EU - Next Generation EU Mission 4 “Education and Research” - Component 2: “From research to business” - Investment 3.1: “Fund for the realisation of an integrated system of research and innovation infrastructures” - Project IR0000032 – ITINERIS - Italian Integrated Environmental Research Infrastructures System - CUP B53C22002150006.

The authors acknowledge the Research Infrastructures participating in the ITINERIS project with their Italian nodes: ACTRIS, ANAEE, ATLaS, CeTRA, DANUBIUS, DISSCO, e-LTER, ECORD, EMPHASIS, EMSO, EUFAR ,Euro-Argo, EuroFleets, Geoscience, IBISBA, ICOS, JERICO, LIFEWATCH, LNS, N/R Laura Bassi, SIOS, SMINO.

How to cite: Catapano, I., Esposito, G., Gennarelli, G., and Soldovieri, F.: Drone based radar technologies for wide rural areas resources exploration: potentialities and challenges, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17346, https://doi.org/10.5194/egusphere-egu25-17346, 2025.

EGU25-18196 | Posters on site | GI1.3

SEAWATCH Project: A year of advancements in Short-Range K-Band Radar for Coastal Monitoring 

Giovanni Ludeno, Pasquale Contestabile, Diego Vicinanza, Matteo Antuono, Caludio Lugni, Ilaria Catapano, Giuseppe Esposito, Carlo Noviello, Francesco Soldovieri, and Gianluca Gennarelli

Coastal regions are crucial for human settlements and economic development. However, their distinctive environmental characteristics, particularly in deltas, bays, and gulfs, render them highly vulnerable to threats such as erosion phenomena and pollution. The effective management of these areas depends on the accurate predictions of wave dynamics and their interactions with the shoreline and seabed. Reliable forecasts require numerical wave propagation models to be initialized with precise data and detailed bathymetric representations, and their accuracy depends on calibration operations using high-quality sea state observations.

Sea state data are typically collected through in-situ sensors, such as buoys and drifters, or remote sensing devices, including radars and video-monitoring systems [1]. Remote sensing technologies are often preferred due to their ability to provide both spatial and temporal information. Among these, ground-based radar systems like High-Frequency and X-band radars have proven effective in retrieving wave spectra and coastal sea state information. However, these systems face notable limitations, including difficulties in acquiring data near the shoreline. Additionally, they are bulky, heavy, and cumbersome, which complicates the deployment stage.

To address these challenges, the Italian PRIN-PNRR 2022 Project SEAWATCH—Short-Range K-Band Wave Radar System Close to the Coast—was launched on November 30, 2023. SEAWATCH focuses on developing an innovative, portable, short-range K-band radar prototype specifically designed for sea state monitoring in nearshore zones. Thanks to its compact size, lightweight design, and low power requirements, the system enables flexible, on-demand surveys, meeting critical safety and environmental management needs in harbors and coastal zones.

This communication outlines the key activities and initial results achieved during the first year of the SEAWATCH project. This last is organized into six milestones, supported by a robust collaboration between research units to ensure efficient knowledge sharing and steady progress. Preliminary here results shown highlight the radar prototype potential to overcome traditional limitations, offering enhanced spatial resolution and real-time monitoring capabilities near the coastline [2]-[4].

Future efforts will focus on further refining the radar prototype and validating its performance across diverse coastal environments.

 

References:

  • P. Neill, M. Reza Hashemi, Chapter 7 - In Situ and Remote Methods for Resource Characterization, Editor(s): Simon P. Neill, M. Reza Hashemi, In E-Business Solutions, Fundamentals of Ocean Renewable Energy, Academic Press, 2018, Pages 157-191.
  • Afolabi, L. A., et al. (2025). Underestimation of Wave Energy from ERA5 Datasets: Back Analysis and Calibration in the Central Tyrrhenian Sea. Energies, 18(1), 3.
  • Ludeno, G., Antuono, M., Soldovieri, F., & Gennarelli, G. (2024). A Feasibility Study of Nearshore Bathymetry Estimation via Short-Range K-Band MIMO Radar. Remote Sensing16 (2), 261.
  • Ludeno, G.; Esposito, G.; Lugni, C.; Soldovieri, F.; Gennarelli, G. A Deep Learning Strategy for the Retrieval of Sea Wave Spectra from Marine Radar Data.  Mar. Sci. Eng.202412, 1609.

 

Acknowledgment: This work was supported and funded by the European Union—NextGenerationEU PNRR Missione 4 “Istruzione e Ricerca”—Componente C2 Investimento 1.1, “Fondo per il Programma Nazionale di Ricerca e PRIN—SEAWATCH—Short-rangE K-bAnd Wave rAdar sysTem Close to tHe coast CUP B53D23023940001, and partially funded by the research project STRIVE—La scienza per le transizioni industriali, verde, energetica CUP B53C22010110001.

How to cite: Ludeno, G., Contestabile, P., Vicinanza, D., Antuono, M., Lugni, C., Catapano, I., Esposito, G., Noviello, C., Soldovieri, F., and Gennarelli, G.: SEAWATCH Project: A year of advancements in Short-Range K-Band Radar for Coastal Monitoring, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18196, https://doi.org/10.5194/egusphere-egu25-18196, 2025.

EGU25-18356 | ECS | Posters on site | GI1.3

Applicability of cheap and lightweight magnetic sensors to geophysical exploration 

Filippo Accomando and Giovanni Florio

 In recent years, there was a notable technological advancement in geophysical sensors. In the case of magnetometry, several sensors were used having the common feature to be miniaturized and lightweight, thus idoneous to be carried by UAV in drone-borne magnetometric surveys. Moreover, such sensors have the common feature to be very cheap, so that it is in principle very easy to have the resources to combine two or three of them to form gradiometers. Nonetheless, another common feature is that their sensitivity ranges from 0.1 to about 200 nT, thus not comparable to that of alkali vapor, standard flux-gate or even proton magnetometers. However, their low-cost, small volume and weight remain as very interesting features of these sensors. In this communication, we want to explore the range of applications of small tri-axial magnetometers commonly used for attitude determination in several devices. We compare the results of ground-based surveys performed with conventional geophysical instruments with those obtained using these sensors.

 

How to cite: Accomando, F. and Florio, G.: Applicability of cheap and lightweight magnetic sensors to geophysical exploration, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18356, https://doi.org/10.5194/egusphere-egu25-18356, 2025.

EGU25-18926 | ECS | Orals | GI1.3

Remote Sensing for Volcanic Eruptions and Earthquake Emergency Management Strategies in Developing Countries 

Tesfaye Tessema, Elias Lewi, and Fabio Tosti

Volcanic eruptions and earthquakes present significant challenges to developing countries, where limited monitoring infrastructure restricts effective risk mitigation efforts. Satellite remote sensing observations offer essential information, including surface deformation and thermal anomalies, for hazard assessment, early warning, and emergency response. These satellite-based observations enable comprehensive spatial and temporal monitoring, utilising both publicly available medium-resolution and commercial high-resolution datasets. Over the past decade, Sentinel radar and optical observations have been employed in areas with limited in-situ measurement capabilities[1]. Nonetheless, the utilisation of these datasets in developing countries is frequently hampered by insufficient computational and analytical resources.

This study examines the role of remote sensing in strengthening disaster risk management within resource-constrained contexts. We propose a collaborative framework that utilises satellite remote sensing data processing Centres in developed countries to assist developing nations in analysing pre-, during, and post-crisis events. Moreover, we advocate for engaging with space agencies to enhance satellite tasking during crisis observation, thereby improving our understanding of the event’s driving mechanisms. We highlight the critical role of remote sensing through a case study of recent seismic and volcanic activity in the Main Ethiopian Rift, specifically between the Fentale and Dofen volcanoes[2]. While national seismic and geodetic networks provide data on large and medium-magnitude earthquakes and significant deformations, they cannot detect low-magnitude precursory events or local deformations due to their proximity to volcanic centres. Furthermore, the installation of temporary monitoring facilities is often constrained by various limitations. Remote sensing bridges this gap by offering detailed data to support local research, inform timely decision-making, and strengthen crisis management. The crises have impacted under-resourced regions, the primary import-export corridor, and nearby urban centres, including Addis Ababa, where rapid urbanisation has raised safety concerns. This study underscores the necessity of integrated remote sensing solutions and international collaboration to enhance resilience and mitigate risks in disaster-prone areas.

Keywords: Sentinel, Main Ethiopian Rift, Fentale Volcano, Developing Countries, Emergency Management

 

Acknowledgements

The Authors would like to express their sincere thanks and gratitude to the following trusts, charities, organisations and individuals for their generosity in supporting this project: Lord Faringdon Charitable Trust, The Schroder Foundation, Cazenove Charitable Trust, Ernest Cook Trust, Sir Henry Keswick, Ian Bond, P. F. Charitable Trust, Prospect Investment Management Limited, The Adrian Swire Charitable Trust, The John Swire 1989 Charitable Trust, The Sackler Trust, The Tanlaw Foundation, and The Wyfold Charitable Trust.

 

References

[1] Tessema, T. T., Biggs, J., Lewi, E., & Ayele, A. (2020). Evidence for active rhyolitic dike intrusion in the northern Main Ethiopian Rift from the 2015 Fentale seismic swarm. Geochemistry, Geophysics, Geosystems, 21, e2019GC008550. https://doi.org/10.1029/2019GC008550

[2] Derek Keir, Alessandro La Rosa, Carolina Pagli, et al. (2024). The 2024 Fentale Diking Episode in a Slow Extending Continental Rift. ESS Open Archive DOI: 10.22541/au.172979388.80164210/v1

How to cite: Tessema, T., Lewi, E., and Tosti, F.: Remote Sensing for Volcanic Eruptions and Earthquake Emergency Management Strategies in Developing Countries, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18926, https://doi.org/10.5194/egusphere-egu25-18926, 2025.

EGU25-19565 | ECS | Orals | GI1.3

Innovative Geothermal Mining through Membrane Technologies 

Bruno Marco Inzillo, Sergio Santoro, Efrem Curcio, and Salvatore Straface

Critical raw materials (CRMs) are crucial for technological advancements and the global energy transition, especially in sectors such as renewable energy, electronics, and electric mobility. The sustainable and secure management of these materials is increasingly important. Geothermal springs represent a promising source of CRMs, offering valuable materials such as lithium, magnesium, strontium, and boron in addition to clean energy. Depending on where they come from geologically, geothermal springs can have lithium levels that are at least 10 times higher than seawater (0.18 mg/L) and about the same as salt lakes (0.04–3 g/L). The moderate Mg2+/Li+ molar ratio (~35) also shows that the two elements might be better separated, which would allow for more Mg2+ recovery. This study introduces a novel method for the recovery of CRMs from geothermal brines, combining Reverse Osmosis (RO), Nanofiltration (NF), and Membrane Distillation (MD) for efficient separation of water and valuable materials. The experiments are conducted using a synthetic laboratory-reproduced geothermal spring solution, which accurately replicates the pH, temperature, and ionic composition typical of natural geothermal waters. This experimental approach ensures that the results reflect real-world conditions, which is critical for evaluating the feasibility and scalability of the proposed method. The process begins with RO and NF to concentrate the brine and selectively separate multivalent ions (e.g., Mg) from monovalent ions (e.g., Li), leveraging differences in ionic valence. Following this, MD is applied to reduce brine volume and minimize thermal energy consumption, thereby optimizing both water recovery and the concentration of CRMs. A key innovation of this work is the exploitation of the elevated temperature of geothermal brines (> 35°C), which allows the use of MD with minimal external heating. This significantly reduces energy requirements and operational costs. The process minimizes Specific Thermal Energy Consumption (STEC), highlighting its efficiency and sustainability. This method not only enhances the recovery of lithium and magnesium from geothermal springs, but it also offers a cleaner, more sustainable approach to CRM extraction by utilizing renewable geothermal heat.

How to cite: Inzillo, B. M., Santoro, S., Curcio, E., and Straface, S.: Innovative Geothermal Mining through Membrane Technologies, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19565, https://doi.org/10.5194/egusphere-egu25-19565, 2025.

EGU25-19593 | ECS | Orals | GI1.3

Enhancing Hydrological Models with Remote Sensing: A Review of Products, Techniques, and Uncertainties 

Soufiane Taia, Yassine Ait Brahim, Mohammed Hssaisoune, Andrea Scozzari, and Bouabid El Mansouri

Distributed hydrological models are crucial for flood prediction, drought analysis, and water resource monitoring. They are typically calibrated using streamflow observations at the watershed outflow to determine the best parameter values within their common ranges. These models are then applied to analyze management and climate scenarios. However, accurately representing hydrological complexities is challenging due to limited knowledge, data availability, and imprecise measurements. Uncertainties in these models arise from parameters, model structure, calibration processes, and data, especially in regions with scarce data. Consequently, hydrological models require extensive hydro-meteorological data for calibration and validation, which can be costly and time-consuming. Recently, remote sensing techniques advanced hydrological modeling by providing regular sampling of essential variables like precipitation, soil moisture, and evapotranspiration. However, thanks to technological advancements, numerous global and regional remote seeing products for the same variable have become freely available. These products vary in their algorithms, approaches, spatial and temporal resolutions, leading to diverse datasets for the same variable. Therefore, different products can perform differently in terms of parameter estimation, model robustness, and water balance predictions within the same area. However, each product may introduce biases or uncertainties, necessitating modelers to assess their performance and carefully choose the most suitable product for their study objectives. This research reviews commonly used remotely sensed products and the techniques and approaches for integrating them into distributed and semi-distributed hydrological models. Additionally, this review examines the uncertainties associated with different existing products and their performance within hydrological models.

How to cite: Taia, S., Ait Brahim, Y., Hssaisoune, M., Scozzari, A., and El Mansouri, B.: Enhancing Hydrological Models with Remote Sensing: A Review of Products, Techniques, and Uncertainties, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19593, https://doi.org/10.5194/egusphere-egu25-19593, 2025.

EGU25-19717 | ECS | Orals | GI1.3

Advancing Community-Based Water Quality Monitoring through Low-Cost Open-Source Optical Sensors and Data Integration 

Riccardo Cirrone, Amedeo Boldrini, Alessio Polvani, Xinyu Liu, and Steven Loiselle

To meet European (WFD) and International objectives (SDGs), there is a growing demand for water quality data with elevated spatial and temporal resolution. This has been an ongoing process, achieved by integrating data from governmental agencies with community-based monitoring initiatives (crowdsensing). Community-based monitoring has proven effective in addressing information gaps in managing and monitoring aquatic ecosystems, particularly in small rivers that often lack agency monitoring. However, there are still challenges regarding the reliability of such data. To fill this gap, there is an urgent need to develop affordable, reliable, and open-source instrumentation for water quality monitoring. These instruments should also comply with the recent European guidelines on the use of toxic substances in technology development.

This study presents the development and validation of a RoHS directive-compliant, open-source, low-cost optical sensor for detecting nitrates and phosphates in community-based monitoring initiatives. The sensor setup takes advantage of light-emitting diodes (LED) as light sources and a commercial ambient light detector. A second light sensor positioned at a 90° angle is employed for scattering correction. All components are managed by a Raspberry Pi Zero W microcomputer and housed in a custom 3D-printed poly(lactic acid) case. The device enables data collection, including GPS coordinates, with results stored offline or transmitted in real-time through Wi-Fi. The sensor’s analytical performance was evaluated in both laboratory and field conditions using reference materials and river samples. Results demonstrated accurate and repeatable measurements which were shown to increase resolution and precision compared to standard colorimetric methods. To promote accessibility and replication, the 3D-box CAD model, software, and usage guidelines are freely available online.

How to cite: Cirrone, R., Boldrini, A., Polvani, A., Liu, X., and Loiselle, S.: Advancing Community-Based Water Quality Monitoring through Low-Cost Open-Source Optical Sensors and Data Integration, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19717, https://doi.org/10.5194/egusphere-egu25-19717, 2025.

EGU25-20136 | ECS | Posters on site | GI1.3

Towards the Integration of GPR and Magnetic Data for the Study of Urban and Rural Areas 

Francesco Mercogliano, Andrea Barone, Andrea Vitale, Giuseppe Esposito, Pietro Tizzani, and Ilaria Catapano

Among Non-Destructive Testing (NDT) methods, Ground Penetrating Radar (GPR) and magnetic surveys are among the most widely used techniques for various applications, including geo-environmental, archaeological, geotechnical, and engineering purposes. Their success is attributed to factors such as cost-efficiency, versatility, and data collection capabilities. Additionally, both methods enable the detection of buried targets through their respective magnetic and electromagnetic properties. Integrating the results from these two methodologies can yield excellent outcomes for an in-depth analysis of the investigated environment and significantly enhance the detection capabilities for anomaly sources.

This study presents preliminary results on the integration of simulated GPR and magnetometric data for a representative scenario. Advanced imaging techniques, including the Depth from Extreme Points (DEXP) method for magnetic data and the microwave tomography approach for GPR data, were applied to produce an initial high-resolution visualization of the simulated target.

Building on these results, an arithmetic integration approach was used to merge the two datasets into a single image, enhancing the interpretation of the anomaly source, including its morphology, position, and depth.

These preliminary results demonstrate the potential of this workflow, based on the arithmetic integration of these datasets, to provide more accurate and detailed subsurface models. This approach paves the way for real-world applications, and further developments aim to refine it for broader geophysical purposes.

Acknowledgments: the project ITINERIS "Italian Integrated Environmental Research Infrastructure Systems" (IR0000032), which funded the research

How to cite: Mercogliano, F., Barone, A., Vitale, A., Esposito, G., Tizzani, P., and Catapano, I.: Towards the Integration of GPR and Magnetic Data for the Study of Urban and Rural Areas, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20136, https://doi.org/10.5194/egusphere-egu25-20136, 2025.

Microwave links from cellular communication networks have been proposed as an opportunistic source of precipitation data more than two decades ago. The first scientific studies demonstrating the potential of this ground-based remote sensing technique, in particular for areas around the world lacking dedicated rainfall observation networks, were published more than 15 years ago. Since then, a small but dedicated community of scientists and engineers working at universities, national meteorological services, engineering firms, mobile network operators and telecommunication equipment manufacturers has been making significant progress in turning this promise into a reality. In the meantime, numerous papers and reports have been published, conference presentations have been given and courses have been delivered. However, real-time access to high-resolution rainfall information from commercial microwave link networks over large continental areas is still a dream. How far have we come after more than 20 years of research and development? What does the future have in stall for the hydrological and meteorological communities? What should be done to turn this dream into a reality? Finally, which other hydrometeorologically relevant variables could potentially be retrieved using received signal levels from commercial microwave links? This sollicited presentation will attempt to provide some preliminary answers to these questions.

How to cite: Uijlenhoet, R.: Hydrometeorological Monitoring using Microwave Links from Cellular Communication Networks: Opportunities and Challenges, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20151, https://doi.org/10.5194/egusphere-egu25-20151, 2025.

EGU25-20810 | Posters on site | GI1.3

Building a Smart Dendrometer: Calibration and Field Deployment of a linear magnetic driven IoT Sensor for Real-Time Radial Growth Assessment 

Luca Belelli Marchesini, Jim Yates, Francesco Renzi, and Riccardo Valentini

Technological advancements in forest digitization have revolutionized real-time monitoring of tree ecophysiological processes. Direct measurement sensors, such as dendrometers, sap flow sensors, and spectrometers, enable high-resolution insights into tree function and growth. Here, we present a novel dendrometer designed to monitor radial stem increment using a Hall effect-based linear magnetic encoder system integrated into an IoT-enabled platform.

The dendrometer employs a commercially available linear magnetic encoder chip (AMS OSRAM GmbH) that operates without physical contact, ensuring low power consumption and long-term monitoring suitability. Key design components include a linear arm, sensor housing, rail, magnetic tape, and chip braces. Calibration was conducted using a stepper motor for linear movements at 0.1 mm increments, capturing 100 data points per step in four replicates. Regression analysis demonstrated high accuracy, with an R² of 0.99 and an RMSE of 0.05 mm. Temperature sensitivity tests (0–40°C) revealed minimal impact on sensor performance.

Field tests over one growing season involved four dendrometers installed on specimens of spruce (Picea abies (L.) H.Karst)) and silver fir (Abies alba Mill.). Seasonal radial growth patterns captured by the devices aligned closely with established static UMS D1 diameter belt measurements, demonstrating their capacity to detect both long-term trends and short-term diel stem oscillations.

This study highlights the potential of an IoT-driven dendrometer for capturing high-resolution radial growth data, offering insights into tree physiology and forest responses to environmental changes. Future development should focus on enhancing measurement precision through design optimization and improved access to power width modulation components in the AS3511 chip. This dendrometer represents a promising tool for advancing forest monitoring and understanding the impacts of climate change on tree growth dynamics.

How to cite: Belelli Marchesini, L., Yates, J., Renzi, F., and Valentini, R.: Building a Smart Dendrometer: Calibration and Field Deployment of a linear magnetic driven IoT Sensor for Real-Time Radial Growth Assessment, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20810, https://doi.org/10.5194/egusphere-egu25-20810, 2025.

EGU25-20884 | Posters on site | GI1.3

A Cost-Effective Automatic Chamber for Permanent CH4 and N2O Assessments inWetland Environments 

Milan Shay Kretzschmar, Maren Dubbert, Mathias Hoffmann, Milos Bielcik, Joana Bergmann, and David Dubbert

Wetland ecosystems exhibit large spatial and temporal variability in terms of greenhouse gas (GHG) fluxes, necessitating new technologies to ensure that they are well-monitored. Both manual and automated chamber-based approaches are currently costly and thus limited either in spatial or temporal resolution. Following on from Wang et al. (2022), we propose a new, inexpensive autochamber (TraceCatch) for long-term outdoor installation. Costs for one unit are less than 800€ in total, making it affordable and scalable for long-term ecological research, also in lower income countries such as the global south. The system is based on gathering gas samples over two weeks into four gas bags on a high-frequency sampling schedule. TraceCatch is controlled using an Arduino Uno, connected to a peristaltic pump for sampling of chamber headspace air as well as a number of sensors for air temperature and humidity (SHT-41), air pressure (BMP280), and CO2 concentrations (K30FR; 0–5,000 ppm, 30 ppm resolution). The latter are used to track the sealing condition of the chamber. We validated the system using defined injection amounts of technical gas (100% CO2). In addition, the system was applied to measure GHG fluxes from three wetland cores placed inside three ecotrons (UGT EcoLab flex, manufactured by Umwelt-Geräte-Technik GmbH, Germany). Gas samples were collected 4 times a day for 2 weeks during a 1 hour chamber closure time at t0, t20, t40, t60 and subsequently analyzed using gas chromatography (Nexis GC-2030, manufactured by Shimadzu Corporation, Japan). Average GHG fluxes determined over the two-week period were then compared to single measurements obtained using multi-gas sensors (LI-COR LI-7820 and LI-7810 analyzers, manufactured by LI-COR Biosciences, USA). If adopted, the system’s low cost, scale and robustness for permanent field deployments could help improve wetland GHG monitoring, offering a cost-efficient and practical alternative to traditional methods for global-scale biogeochemical cycle assessments.

How to cite: Kretzschmar, M. S., Dubbert, M., Hoffmann, M., Bielcik, M., Bergmann, J., and Dubbert, D.: A Cost-Effective Automatic Chamber for Permanent CH4 and N2O Assessments inWetland Environments, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20884, https://doi.org/10.5194/egusphere-egu25-20884, 2025.

EGU25-21862 | Posters on site | GI1.3

TreeTalker Cyber: A Multi-Sensor, Low-Cost IoT Platform for Real-Time Monitoring of Tree Ecophysiology 

Francesco Renzi, Jim Yates, Valerio Coppola, Salvatore Riggi, Maria Vincenza Chiriacò, and Riccardo Valentini

The Earth is a complex ecosystem and each element is strictly linked with the others. It is often required to collect data on multiple aspects variously related to the main phenomenon in order to understand its mechanism. Moreover, the increasing use of machine learning algorithms requires the creation of new, reliable and extensive dataset in order to obtain significant results. The increasing demand for accurate, real-time monitoring of tree ecophysiological parameters presents challenges in developing affordable and efficient technologies, in particular in difficult environments such as mountains. TreeTalker Cyber, an innovative IoT platform, addresses these needs by integrating multiple sensors into a single, cost-effective device capable of measuring radial growth, radiation intensity below the canopy across 26 spectral bands, sap-flow, microclimate data, and trunk inclination. This presentation explores its capabilities, practical applications, and potential to transform forest monitoring globally. The use of a single platform to collect all the aforementioned parameter greatly reduces the cost of the equipment per collected parameter providing at the same time all main information required to evaluate the status of a tree, improving the maintenance of the network at the same time. The device is equipped with an NB-IoT or LoRaWAN transmission module to transmit collected data and make them available remotely. A comprehensive description of the platform and real field data are presented along with the technologies used for data transmission and storage with their strength and weaknesses. The OGC SensorThings API is also briefly described along with FROST (FRaunhofer Opensource SensorThings-Server) as an alternative to efficiently store IoT data and make them compliant with the FAIR principles, making them usable by both scientific and public communities. The creation of a dataset of trees ecophysiological parameters will help deepening the knowledge and understanding of forests around the world. TreeTalker Cyber lays the groundwork for advancing forestry research, providing fine-scale data as ground truth for forestry models and a starting point for future scenarios predictions, in particular when based on machine learning algorithms.

How to cite: Renzi, F., Yates, J., Coppola, V., Riggi, S., Chiriacò, M. V., and Valentini, R.: TreeTalker Cyber: A Multi-Sensor, Low-Cost IoT Platform for Real-Time Monitoring of Tree Ecophysiology, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21862, https://doi.org/10.5194/egusphere-egu25-21862, 2025.

Anatolia is a geography that has experienced major natural disasters from ancient times to decay due to its geological location. In this context, Anatolia has always attracted the attention of researchers. The earthquakes that occurred in 6 provinces of Turkey, namely Anatolia, on February 6, 2022, and caused great loss of life and property, the re-emergence of the earthquake explosion in Anatolia. We, archaeologists, have been exposed to major earthquakes and climates from ancient times to decay, and situations that can be defined as natural have caused great losses. The Hittites, Assyrians, Hellenes, Romans, and societies before and after these civilizations, who continued their existence in Anatolia in ancient times, suffered great material and spiritual losses as a result of natural disasters experienced in the geography of Anatolia, and the ancient geological and climatological documentation of Anatolia has been documented. This is possible, the earthquakes and climatic conditions that occurred in Anatolia from ancient times to decay and are included in historical records due to its service location will be included, and it will be discussed how these earthquakes and climatic events will end archaeological settlements in ancient times and today.

 

 

How to cite: Yüksel Özer, F.: Natural disasters that occurred in ancient times in Anatolia and the damage they caused to ancient settlements, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1907, https://doi.org/10.5194/egusphere-egu25-1907, 2025.

Architectural heritage in the African context, as a domain of cultural heritage, frequently encounters substantial obstacles for conservationists and custodians due to the lack of fully documented current conditions or as-built blueprints, which serves as the initial obstacle. Most architectural heritage buildings constructed prior to and during the colonial era lack documentation; traditional heritage structures were created through generational knowledge, while colonial buildings were built using imported knowledge, which largely dissipated after independence.
The second primary difficulty is the absence of documented social narratives pertaining to these heritage buildings. Numerous heritage buildings in Africa has profound cultural significance that is gradually being eroded owing to insufficient recording. This essay will introduce a prototype project in Porto-Novo, Benin, wherein the author utilizes local social engagement and digital technologies to chronicle Afro-Brazilian or Aguda architecture, a vanishing architectural heritage in Benin. Afro-Brazilian architecture is a construction style created by formerly enslaved Africans who resettled in the Bight of Benin countries following the abolition of slavery in Brazil. This settlement developed a distinctive architectural style that amalgamated Brazilian and native African influences, particularly Yoruba, significantly affecting the urban morphology of Benin.
The project utilizes LiDAR scanning, photogrammetry, and geolocation technologies to digitize heritage structures and develop interactive immersive interfaces that facilitate engagement with and access to this valuable architectural heritage.

H. Killion Mokwete is Assistant Professor at Northeastern and UK-trained and registered Architect (RIBA-chartered Architect & Urban Designer) and Co-Founder of the community-based design startup Social Impact Collective (SIC). He teaches various design studios both at undergraduate and graduate level and is currently undertaking multidisciplinary research initiative in Benin with local historians at the Ecole du Patrimoine Africain - School of African Heritage (EPA), Benin, Porto-Novo.

How to cite: Mokwete, H.: Digitizing Afro Brazilian Architectural Heritage buildings in Benin through LiDAR technology and social participation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2907, https://doi.org/10.5194/egusphere-egu25-2907, 2025.

EGU25-4316 | ECS | Orals | CL3.2.7

From Polygon to Prediction: A Request-Driven Architecture for Disaster Mapping and Impact Assessment  

Luca Barco, Gaetano Chiriaco, Tommaso Monopoli, Edoardo Arnaudo, and Claudio Rossi

Disasters pose significant threats to cultural heritage and natural landscapes. To mitigate damage and plan effective recovery actions, it is crucial to conduct precise impact assessments. 

This work presents a service that offers an innovative, adaptable and scalable solution, integrating remote sensing and delineation models to map catastrophic events and estimate the elements affected within the area of impact. By leveraging satellite imagery and advanced AI-based mapping models, the service is tailored to delineate and estimate the severity of the hazards, providing additional information about population, infrastructures, constructed elements (potentially including culturally significant structures) and land cover. 

The primary utility of the service lies in its ability to map catastrophic events, i.e. fires, floods and landslides with high accuracy. By delineating the affected areas, stakeholders can gain immediate insights into the extent and nature of the disaster. In addition to this core functionality, the service also provides valuable metadata about the elements within the impacted area, enabling a deeper understanding of the disaster’s impact. 

Cultural heritage sites, particularly those integrated into natural landscapes, are vulnerable to various natural phenomena. Assessing the extent of the damage requires accurate and timely information about the affected areas. Our approach is rooted in geospatial technologies, providing an automated workflow that begins with the input of a polygon defining the area of interest and a specific period. From there, the system downloads the best high-resolution remote sensing images available and runs delineation models designed for disaster mapping. These models enable the identification of impacted cultural and natural assets with high precision. 

A unique aspect of the service is its adaptability. While current assessments are often based on standardized taxonomies, these classifications were generally not designed to explicitly characterize cultural heritage. The service allows for the integration of site-specific base maps, enabling a more refined analysis tailored to the unique attributes of cultural sites and their surrounding landscapes. 

Impact assessments are a cornerstone for planning recovery actions post-disaster. service’s ability to integrate diverse datasets ensures that assessments are not only accurate but also actionable. By providing insights into the damage sustained by cultural heritage and natural landscapes, stakeholders can make informed decisions about restoration priorities and resource allocation. 

Incorporating cultural heritage and natural landscapes into disaster impact assessments is a practical necessity for preserving our shared history and identity. By leveraging remote sensing, advanced delineation models, and adaptable taxonomies, the service provides a robust tool for understanding and mitigating the impacts of disasters.

How to cite: Barco, L., Chiriaco, G., Monopoli, T., Arnaudo, E., and Rossi, C.: From Polygon to Prediction: A Request-Driven Architecture for Disaster Mapping and Impact Assessment , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4316, https://doi.org/10.5194/egusphere-egu25-4316, 2025.

EGU25-4438 | ECS | Posters on site | CL3.2.7

Historic buildings under the impact of climate change: insights from geoelectric field monitoring 

Wiebke Lehmann, Lukas Römhild, Wolfgang Gossel, and Peter Bayer

Extreme weather events driven by climate change, such as floods and droughts, are damaging the structural stability of historic buildings in Central Germany by causing moisture retention and soil desiccation. The alternating wet and dry periods lead to cracks in walls and subsidence from falling groundwater levels. Understanding the impact of these conditions on regional groundwater dynamics and building materials is crucial as droughts and floods are expected to increase in the coming years.
As part of this study, three geoelectric field campaigns with a total of 17 profiles are being carried out between April 2024 and April 2025 at five different field sites of monuments in the federal states of Saxony and Saxony-Anhalt. For investigating seasonal and weather-dependent fluctuations in groundwater conditions, transient trends are observed by repeated electrical resistivity tomography (ERT) measurements. These provide insights into hydrological changes in the subsoil, and thus information on how weather events can affect different layers of the soil as well as foundation structures. In addition to the geoelectrical investigations, 14 groundwater wells are being drilled to a depth of around 10 m to monitor the fluctuations in the groundwater level over time. Furthermore, complementary laboratory tests are being conducted to characterize the soil properties, allowing a reliable interpretation of the ERT inversion results.
Preliminary results indicate that layers down to 25 m depth can be affected by weather-dependent variations in resistivity, depending on the hydraulic properties of the soil material at the respective site. Despite the elevated precipitation during the summer months of June and July, the topsoil underwent significant drying by November 2024, leading to a reduction in the groundwater level and subsequent saturation of the deeper soil layers. Ongoing continuous measurements shall provide further insights.

How to cite: Lehmann, W., Römhild, L., Gossel, W., and Bayer, P.: Historic buildings under the impact of climate change: insights from geoelectric field monitoring, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4438, https://doi.org/10.5194/egusphere-egu25-4438, 2025.

EGU25-4992 | Orals | CL3.2.7

Assessing the Exposure of Coastal Cultural Heritage Sites to Sea Level Rise Phenomena in the EU Mediterranean Countries using open access data 

Sevasti Chalkidou, Charalampos Georgiadis, Themistoklis Roustanis, and Petros Patias

The Mediterranean Sea has a long record of cultural heritage sites located near its coast, reflecting each nation’s historical continuum and identity. These monuments also attract tourism and provide financial benefits to local communities. However, they are subject to structural damage and decay exacerbated by climate-change-related phenomena including extreme weather events, sea-level rise, etc. Sea Level Rise (SLR) is a major threat to coastal heritage sites as it can  lead to extensive inundation and soil erosion. SLR projections are constructed by studying representative pathway scenarios (RCP), which try to deliver possible alternatives about the future atmospheric composition.  SLR has escalated from an average of 1. 2 mm/year before 1990 to 3 mm/year between 1993 and 2010, with projections indicating a rise of 1–2 meters by 2100 across different scenarios.

The ongoing Triquetra Project, funded by the European Union, aims to design a toolbox for assessing and mitigating climate-related risks and natural hazards, expected to affect Heritage Sites. A methodology has been developed to evaluate future exposure of coastal heritage sites SLR in EU Mediterranean Countries. This workflow uses open-access data to produce SLR projection maps for 2050 and 2100 based on the IPCC (2019) report for RCP 2.6, 4.5, and 8.5. Four main sources of data were used: a hybrid coastline vector file combining national fine-scale datasets with the European Environment’s Agency (EEA) coastline file, FABDEM as the primary source of elevation information,  the European Ground Motion Vertical Service’s (EGMS) L3 product which measures vertical ground movements using Synthetic Aperture Radar Interferometry (InSAR) data from the Sentinel-1 mission, and, finally, NASA’s Sea Level Projection Tool which provides information on all RCP scenarios. Coastal Heritage Sites and Assets were identified using OpenStreetMap and UNESCO’s Word Heritage Site point layer.

The pre-processing stage of the algorithm involves the projection of all datasets into a common coordinate reference system, the clipping of the data into the area of interest (AOI), defined as a 2km buffer zone from the coastline, and the conversion of EGMS and NASA’s SLR data units to meters. The algorithm proceeds with raster calculations to determine the AOI’s elevation for the target years 2050 and 2100 under different RCP scenarios by adding the elevation values to the EGMS data and subtracting NASA’s SLR projected values. Raster calculations and Boolean algebra are performed to identify sub-areas affected by these scenarios. Finally, spatial queries are conducted to find coastal heritage sites at risk from Sea Level Rise, organized by monument type and country for vulnerability assessment.

The results demonstrate that Greece, France, and Italy are expected to be more affected by SLR phenomena due to their extensive coastline and unique geomorphology, with the impact being more severe on Greece and Italy between 2050 and 2100. Finally, more than 240 heritage sites appear to be at risk primarily on the Greek and Italian coast, including UNESCO sites like Delos, the Medieval City of Rhodes, et al.

How to cite: Chalkidou, S., Georgiadis, C., Roustanis, T., and Patias, P.: Assessing the Exposure of Coastal Cultural Heritage Sites to Sea Level Rise Phenomena in the EU Mediterranean Countries using open access data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4992, https://doi.org/10.5194/egusphere-egu25-4992, 2025.

EGU25-6132 | Orals | CL3.2.7

Value-based and stakeholder-driven complex risk mapping for underwater heritage through Living Labs 

Deniz Ikiz, Paloma Guzman, Cristina Veiga-Pires, Sonia Oliveira, Stella Demesticha, Anna Demetriou-Patsalidou, Paschalina Giatsiatsou, Ionut Cristi Nicu, and Panagiotis Michalis

Climate change is one of the biggest threats to cultural and natural heritage across marine and coastal ecosystems. Multiple risks interact, cascade, and/or compound broader environmental, socio-economic, and cultural impacts on tangible (places, structures, ecosystems, etc.) and intangible heritage attributes (values, socio-economic activities, etc.). These risks arise from exposure, vulnerability, and responses to such impacts. For example, the physical materiality and integrity of underwater cultural properties are threatened by changes in water temperatures and acidity levels, compounded by extreme weather events causing strong waves and currents, which disrupt livelihoods tied to tourism and fisheries and provide conditions for looting and unregulated diving. This study adopts an empirical, value-based, and stakeholder-driven approach to identify, assess, and map these complex risks and their interactions.  

As part of the THETIDA Horizon Europe project that aims to develop an integrated risk monitoring, preparedness, and management mechanism for underwater and coastal heritage sites, the Living Labs methodology has been employed in the pilot sites. Through public-private-people partnerships, the Living Labs engage relevant national and local stakeholders and community groups to identify values, determine impacts, and assess exposure, vulnerability, and responses. This stakeholder-driven complex risk mapping methodology relies on the framework for complex climate change risk assessment that includes response as the fourth determinant of risks, together with hazard, exposure, and vulnerability [1]. In addition, it builds upon the Climate Vulnerability Index (CVI) for World Heritage, which employs a systematic and value-based approach to assess the climate vulnerability of shared values and attributes of cultural and natural properties [2]. Building upon CVI’s two-stepped procedure targeting to assess impacts on heritage values and communities, this complex risk mapping framework adopts a similar process to determine:

  • Risks to heritage values: The heritage values attributed to the sites are identified. Moreover, their vulnerability, exposure to risks, and the impacts of key hazards and climate stressors on the sites are assessed.
  • Risks to heritage communities: The heritage communities (stakeholders) and their socio-economic and cultural connections to the sites are identified. At the same time, their vulnerability, exposure to risks, and collective and/or institutional responses to climate-induced impacts are being evaluated.

This paper will present this innovative complex risk mapping framework and its preliminary implementation results in one of the THETIDA underwater sites. These sites include the Ottoman shipwreck in Paralimni, Cyprus, and the Second World War airplane wreck off the coast of Algarve, Portugal.

The complex risks posed to underwater heritage sites and their interactions remain largely underexplored in the existing literature, limiting the adoption of inclusive strategies to address them. This value-based and stakeholder-driven complex risk mapping framework outlined here enables a comprehensive assessment of risks and impacts on heritage values and communities. While initially tested for underwater sites, this framework provides a systematic methodology that can be applied to all heritage types, making it highly relevant for decision- and policy-makers working to safeguard underwater and coastal heritage.

Acknowledgement: This research has been funded by European Union’s Horizon Europe research and innovation funding under Grant Agreement No: 101095253, THETIDA project.

References:

[1] DOI: 10.1016/j.oneear.2021.03.005

[2] DOI: 10.5070/P536146384

How to cite: Ikiz, D., Guzman, P., Veiga-Pires, C., Oliveira, S., Demesticha, S., Demetriou-Patsalidou, A., Giatsiatsou, P., Nicu, I. C., and Michalis, P.: Value-based and stakeholder-driven complex risk mapping for underwater heritage through Living Labs, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6132, https://doi.org/10.5194/egusphere-egu25-6132, 2025.

EGU25-8771 | Orals | CL3.2.7

CLICapp: A co-created tool for climate adaptation and safety in human tower exhibitions  

Jon Xavier Olano Pozo, Òscar Saladié Borraz, and Anna Boqué-Ciurana

Climate change poses increasing challenges to outdoor cultural events, including human towers (castells) festivals, which demand favourable weather conditions. Human towers, recognised by UNESCO in 2010 as an Intangible Cultural Heritage of Humanity, rely on safe and comfortable conditions for participants and audiences alike. Building on a project developed in 2024, this communication wants to present the development of a climate-smart decision-making tool to enhance the management of casteller exhibitions under evolving climatic conditions. The prototype tool named Castells, Llindars i Informació Climàtica- CLICapp (Human Towers, Thresholds and Climate Information) aims to transform climate data into valuable information for decision-makers to manage the human tower exhibitions better, especially in summer (due to extreme temperatures and high humidity values) but not only.

The project’s groundwork is the study of temperature trends from 1951 to 2023 during the central hours of the day (12–15h) at four significant festivals (Sant Joan in Valls, Festa Major of La Bisbal del Penedès, Sant Magí in Tarragona, and Sant Fèlix in Vilafranca del Penedès). Results highlighted rising thermal stress, with Heat Index values underscoring the growing discomfort for Castellers (Olano et al., 2024). Then, participatory workshops based on the co-creation methodology for climate services (Font et al., 2021) were held with 109 castellers from 10 teams (colles castelleres), offering qualitative and quantitative insights into their perceptions of favourable and adverse weather for castells. These workshops also generated adaptation proposals prioritised by feasibility and importance (Saladié et al., 2025).

This communication will outline the two new steps undertaken in this project: the introduction of real-time measurements using temperature and humidity sensors in 11 urban squares during the summer season, which provided empirical data on thermal conditions of the exhibitions, and the initial insights into transforming all this data in useful information (climate raw data and co-creation insights) into an app. This app prototype aims to convert climate data and the information collected from the squares and participant groups into understandable and actionable insights for decision-makers—whether they are the Castellers, organisers (i.e. City Hall), other stakeholders (medical services, businesses, police, civil defence), or the public. The developing tool wants to integrate near real-time weather forecasts to identify potential risks for specific festival dates and times. Combining these insights with adaptive strategies proposed in the co-creation workshops provides a robust framework for pre-event planning. The advanced monitoring capabilities will allow organisers to receive near real-time updates on key parameters such as temperature, humidity, Heat Index, or co-created indices based on the information gathered during the workshops.

This project advances the adaptive management of outdoor cultural events by ensuring casteller festivals remain safe and sustainable amid climate change while preserving their cultural essence, safeguarding heritage, promoting climate innovation, and prioritising the well-being of participants. This initiative provides a replicable model for other cultural manifestations facing similar climate challenges worldwide. Incorporating climate services into intangible cultural event management combines scientific research and innovation with cultural preservation to protect the identity, ensure the sustainability of traditions under climate stress, and safeguard human health.

How to cite: Olano Pozo, J. X., Saladié Borraz, Ò., and Boqué-Ciurana, A.: CLICapp: A co-created tool for climate adaptation and safety in human tower exhibitions , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8771, https://doi.org/10.5194/egusphere-egu25-8771, 2025.

Underwater cultural heritage (UCH) sites provide insight into past human behavior and history and thus their preservation is crucial. Within the scope of THETIDA, a Horizon Europe project dedicated to developing technologies and methods to protect coastal and underwater cultural heritage, this work aims to predict the physical processes that can put UCH at risk. This risk assessment is applied to a specific site in the Algarve, Portugal where a WWII U.S. B24 bomber plane crashed approximately 3 km offshore Praia de Faro. The plane now sits 21 m deep on the coastal shelf, which consists mainly of sand. The site is exposed to dominant, more energetic waves coming from W-SW and sheltered from less energetic E-SE waves. The mean significant wave height is 0.9 m, but it can rise to above 3 m with the occurrence of storms. As the site is located in the open ocean, a highly energetic environment, the site is subject to risks caused by wave-induced currents and sediment transport. To analyze and predict these risks in real time a numerical framework integrating three operational process-based models was developed. The numerical system is composed of: 1) the wave model SWAN, 2) the hydrodynamic model MOHID, and 3) the sediment transport model MOHID sediment. The operational wave model uses bathymetric data from EMODNET and is forced with wind conditions from the Skiron Atmospheric Modeling and Weather Forecasting Group in Athens and wave conditions at the boundary from the Copernicus Marine Environmental Monitoring Service (CMEMS). The model was calibrated by testing various formulas for the physical parameters attributed to wave propagation. A statistical analysis was completed to determine the best physics formulas to use for the model by comparing the results of each calibration setting with in-situ buoy measurements. SWAN was then two-way coupled to the hydrodynamic modeling system SOMA (Algarve Operational Modeling and Monitoring System), which is powered by MOHID. The coupling mechanism forces the wave model with velocities and water level output from SOMA and forces SOMA with wave results from SWAN. Preliminary results of the coupling revealed that the impact of current velocity and water levels on wave propagation in the study area is negligible in deeper areas, where the observations used for model validation lie. Further investigations are been conducted to analyze the effects of the two-way coupling in nearshore areas such as the location of the B24. The wave-hydrodynamic coupled system is now being used to develop a non-cohesive sediment transport model, which will be used to evaluate in real-time risks on UCH. This forecasting system will be included in the decision support system of the THETIDA platform.

How to cite: Mills, L.: An Operational Numerical Framework for Assessing Risks to Underwater Cultural Heritage, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9465, https://doi.org/10.5194/egusphere-egu25-9465, 2025.

EGU25-12307 | Orals | CL3.2.7 | Highlight

Monitoring Climate Change in Cultural Heritage Sites Through Enhanced Visualisation Experiences and Crowdsourcing  

Kyriacos Themistocleous, Valentinos Evripidou, and Kyriakos Toumbas

One of the most significant consequences of climate change is the threat it poses to cultural heritage sites. The TRIQUETRA project addresses this critical challenge by applying a comprehensive risk assessment framework. This framework integrates both traditional and advanced technologies, including remote sensing and laser-based spectroscopy, to quantify the severity of risks, monitor their progression, and inform effective mitigation strategies.

Climate risks emerge from the interplay of climate hazards, exposure, and vulnerability. Understanding these risks at the site level is essential to ensure the implementation of appropriate adaptation and mitigation measures. Recent research highlights the compounded impacts of climate-induced geo-hazards, such as landslides and earthquakes, which threaten the physical integrity of monuments and the socio-economic systems they support.
Citizen engagement is a core component of the TRIQUETRA project, which includes a dynamic web and mobile platform where visitors actively participate in monitoring cultural heritage sites. The TRIQUETRA application enables citizens and visitors to contribute valuable datasets by capturing and uploading site photos, complementing and enhancing existing 3D models. A backend system assists cultural site authorities in better monitoring sites by providing up-to-date imagery and reports from visitors. Simultaneously, the TRIQUETRA Citizen Engagement Application creates an interactive and enriched experience for visitors through Virtual Reality (VR) and immersive Augmented Reality (AR) technologies. The application offers additional information through VR and AR experiences, allowing users to learn more about critical features at risk, such as areas affected by climate change or structural vulnerabilities. This fosters awareness and encourages preservation efforts.

The Choirokoitia case study demonstrates the application of the TRIQUETRA methodology in monitoring how the site is affected by climate change while also enhancing the visitor experience. Choirokoitia, a UNESCO World Heritage Site, is one of the best-preserved Neolithic sites in the Mediterranean. It represents the Aceramic Neolithic period of Cyprus at its peak, around the beginning of the 9th millennium BCE. Located in the District of Larnaka, about 6 km from the southern coast of Cyprus, the site leverages crowd-sourced information to provide stakeholders with real-time updates on its condition. By comparing uploaded images to a referenced 3D model, authorities gain valuable insights for preservation.

By integrating advanced technologies and community-driven monitoring, TRIQUETRA ensures a holistic approach to safeguarding cultural heritage. The project establishes a replicable framework that enhances risk assessment and promotes active participation in preservation efforts, offering scalable benefits for cultural heritage sites worldwide.

How to cite: Themistocleous, K., Evripidou, V., and Toumbas, K.: Monitoring Climate Change in Cultural Heritage Sites Through Enhanced Visualisation Experiences and Crowdsourcing , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12307, https://doi.org/10.5194/egusphere-egu25-12307, 2025.

EGU25-13403 | Posters on site | CL3.2.7

Establishment of a transdisciplinary monitoring facility in Delos, Greece for the protection of Natural Heritage from the impacts of Climate Change 

Ilias Fountoulakis, Nikolaos S. Melis, Stavros Solomos, John Kapsomenakis, Anastasia Poupkou, Christos Maris, Costas Synolakis, and Christos S. Zerefos and the Delos Observatory team

The Delos archaeological site, inscribed on the UNESCO World Heritage Site List, is situated on a small rocky island in the center of the Aegean Sea. This uninhabited island boasts of monuments with immense significance to human civilization and it is set within a pristine natural landscape. Delos is increasingly vulnerable to risks due to climate change and geodynamic events, which together endanger its cultural and natural heritage. Recently, a multi-hazard environmental monitoring facility has been established in Delos, incorporating climate and numerical prediction modelling, as well as satellite-based and in-situ real-time monitoring of various seismic, atmospheric, and oceanographic parameters. In addition to providing an overview of the overall facility, we discuss the potential long-term changes in atmospheric parameters such as air temperature, and precipitation along with sea level, that could impact the monuments and the landscape in the future, for different socioeconomic scenarios. Furthermore, we discuss how state-of-the-art models have been downscaled and optimized to forecast meteorological conditions, air quality, and wave activity in the Delos area. Local monitoring of earthquake activity and how it is incorporated into the National Seismic Network, as well as measurements of atmospheric and oceanic parameters are also discussed. The project is a groundbreaking initiative aimed at formulating policies and strategies to promote sustainable growth in the economy, tourism, and culture. It also serves as a model for strengthening the resilience of cultural heritage against natural hazards and risks, as well as a pilot program that aims to be applied to other monuments in Greece and abroad with the support of international organizations (e.g., UNESCO, ICOMOS, Europa Nostra, etc.).

Acknowledgments: This work has been performed in the framework of the project: “Development and installation of an integrated system for the monitoring of the impacts of climatic change on the monuments of Delos” that has been funded by benefit foundations of "Protovoulia ‘21“.

How to cite: Fountoulakis, I., Melis, N. S., Solomos, S., Kapsomenakis, J., Poupkou, A., Maris, C., Synolakis, C., and Zerefos, C. S. and the Delos Observatory team: Establishment of a transdisciplinary monitoring facility in Delos, Greece for the protection of Natural Heritage from the impacts of Climate Change, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13403, https://doi.org/10.5194/egusphere-egu25-13403, 2025.

EGU25-15505 | Posters on site | CL3.2.7

DInSAR analysis for slope instability monitoring due to Climate Change: CUZCO and Machu Picchu case study. 

daniele spizzichino, federica ferrigno, gabriele leoni, and francesco menniti

Andean plateau in Peru and its World Heritage sites are particularly affected by the impacts of climate change. The sacred Valley Archaeological Site around the city of Cuzco, a UNESCO World Heritage Site, is exposed to significant geological risks due to recurrent landslides induced and worsened by climate change effects that threaten its structural integrity, security and exploitation. The Machu Picchu Historic Sanctuary was built on Upper Permian-Lower Triassic (250–300 Ma) igneous rocks, primarily plutonic, which form the Vilcabamba Cordillera's backbone (from 2000m since 6000m a.s.l.) These intrusive formations, oriented ONO–ESE, constitute the elevated regions of the Eastern Cordillera. The area is dominated by a batholith composed mainly of granite and granodiorite, with medium-textured basic granite prominently outcropping within the citadel. The Machu Picchu site and all the sacred valley of Cuzco its surroundings are characterized by instability phenomena driven by complex geomorphological and structural/tectonic conditions worsened by the effects induced at altitude by the climate change (melting of the permafrost, heavy rainfall and increase in temperature). The above mentioned phenomena are exacerbated by the interplay of primary discontinuity families, resulting in recurring processes such as planar slides, rockfalls, topples, debris slides, debris flows, and avalanches. The present work shows the application of Differential Interferometric Synthetic Aperture Radar (DInSAR) technique to measure slow, non-catastrophic morphological changes with millimeter-scale precision. A previous interferometric satellite analysis work carried out in the early 2000s to test the general stability of the Inca Citadel has been resumed and updated. The analysis captures both long-term and seasonal processes triggered by diverse causative factors, enabling informed planning of mitigation strategies. Specifically, DInSAR data processing was conducted for the Machu Picchu archaeological area and for the wider Cusco area, complemented by direct field surveys to validate the results (November 2024). Multi-temporal SAR images from the Sentinel-1 constellation (C-band radar) were processed using advanced DInSAR techniques to generate ground displacement measurement points. The spatial distribution and correlation of these measurements with slope instability and structural damage were analyzed, revealing ground deformation trends from January 2020 to August 2024. Preliminary results indicate that the citadel exhibits average ground and structural displacement of less than 1 mm/year substantially negligible. However, localized analyses highlight distinct patterns of small-scale displacement in the Grupo de las Tres Puertas with slight brick detachment and in the Upper Plaza and Eastern Citadel sector showing relative subsidence compared to adjacent areas, suggesting potential movements of the eastern flank. Monitoring systems (remote and in situ) are recommended. The use of Sentinel-1 DInSAR data provided critical insights into the interaction between ground displacement and archaeological structures. It facilitated the identification of potentially unstable areas, detected anomalies, and traced ground displacement accelerations over time. Displacement anomalies and weather-climate anomalies over time, highlights the effects of the latter on the spatial-temporal increase of instability phenomena. These findings underscore the utility of DInSAR as a powerful tool for addressing preservation of intervention on CH threatened by slope instability, offering data-driven approaches for damage prevention and site management.

How to cite: spizzichino, D., ferrigno, F., leoni, G., and menniti, F.: DInSAR analysis for slope instability monitoring due to Climate Change: CUZCO and Machu Picchu case study., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15505, https://doi.org/10.5194/egusphere-egu25-15505, 2025.

EGU25-16404 | Orals | CL3.2.7

Safeguarding the Past: Monitoring Climate Change at Kalapodi Sanctuary through the TRIQUETRA Project 

Artemios Oikonomou, Angelos Sotiropoulos, Penelope Gourgouleti, and Themistoklis Bilis

Kalapodi arcaheological site is located in central Greece, in the region of present-day Fthiotis consisting of a complex of temples and surrounding remains. It comprises a very important sanctuary, being among the most significant of ancient Phokis, providing crucial insights into Greek religious practices and architectural forms from the Mycenaean to the Classical periods. The archaeogical site in Kalapodi has been the focus of extensive cultural heritage management efforts by the German Archaeological Institute (DAI) since 2017.

As a case study in the TRIQUETRA program, funded by the EU Horizon Europe research and innovation program (GA No. 101094818), this site exemplifies the challenges posed by climate change on cultural heritage. TRIQUETRA project aims to develop an integrated methodological model to safeguard archaeological remains, such as those at Kalapodi, from environmental risks and mainly frost. Central to the project is the creation of an evidence-based assessment platform for precise risk stratification, coupled with a comprehensive database of mitigation measures.

In this paper we would like to leverage environmental data and materials analysis from Kalapodi, so as to quantify the impacts of climate change and propose tailored preservation strategies. These include assessing the effects of frost on ancient structures and implementing preventative measures to ensure their long-term stability. To achieve this a pilot site has been designed and constructed on which several monitoring equipment has been attached to understand the influence of environmental conditions on the pilot and hence the ancient monument. The acquired knowledge and the methodology followed highlights the importance of combining scientific research and heritage management to address climate-related challenges and protect cultural heritage for future generations.

How to cite: Oikonomou, A., Sotiropoulos, A., Gourgouleti, P., and Bilis, T.: Safeguarding the Past: Monitoring Climate Change at Kalapodi Sanctuary through the TRIQUETRA Project, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16404, https://doi.org/10.5194/egusphere-egu25-16404, 2025.

The development of an Agent-Based Model (ABM) has proven highly effective for analyzing how the behavior of different agents leads to aggregated phenomena. Despite the challenges in creating such a model—including conceptualization, agent definition, relationship establishment, behavior design, programming, testing, validation, and reporting—the process allows for valuable testing and rethinking of strategies for enhancing the resilience of cultural landscapes, as the results offer significant insights into phenomena like drought. While not predictive, the observed trends can inform general analysis and highlight key areas for action to achieve specific goals. The RescueMe project developed an ABM that simulates three types of administration and underscores the impact of decision-making on territorial resilience, significantly influenced by timely policies and actions. The primary goal of the model is to simulate how farmers, agricultural plots, and decision-makers interact with each other and their environment, particularly under varying drought conditions. The model tests the hypothesis that decision-makers can intervene to mitigate the effects of drought by creating mechanisms that enhance plot resilience and/or attract new farmers safeguarding the values of the cultural landscapes. In this way, the ABM aims to develop a reflection and awareness-raising tool to allow cultural landscapes to consider the consequences of different climate change adaptation measures and behaviors. The impact chains co-created with the project case studies have been used as a basis for the modeling. The impact chain of drought on agriculture (impact of specific climatic hazards on a given sector) was selected due to its importance for a significant number of cultural landscapes, and the organigraphs created during the early stages of the project were used to help define the agents. The scenarios generated with the ABM simulate the impact of the behavior of agents on landscape resilience and potentially inform the definition of a serious game.

How to cite: Egusquiza, A., Cantergiani, C., and Villanueva, A.: Agent-Based Modeling for analyzing the climate resilience and decision-making impact on drought dynamics in Cultural Landscapes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17815, https://doi.org/10.5194/egusphere-egu25-17815, 2025.

EGU25-18452 | ECS | Posters on site | CL3.2.7

A Multi-Scale Framework for Flood Risk Assessment in Cultural Heritage Sites: The Apollo Temple in Aegina 

Marcos Julien Alexopoulos, Theano Iliopoulou, Denis Istrati, Sofia Soile, Styliani Verykokou, Charalabos Ioannidis, and Demetris Koutsoyiannis

Preserving cultural heritage sites demands risk management strategies that capture site-specific vulnerabilities at fine spatial resolutions. The present study introduces a novel framework for flood risk assessments that bridges large-scale hydrological modeling and sub-meter-level hydraulic simulations to provide enhanced insights into potential impacts. Our approach employs state-of-the-art Rain-on-Grid (RoG) hydraulic simulations, targeted field data collection, and high-resolution geometric documentation using UAV imagery and GNSS ground control points to account for detailed terrain characteristics.

Within the scope of the Horizon Europe TRIQUETRA Project, we apply this framework to the Apollo temple in the archaeological site of Kolona on Aegina Island, Greece. A total of 945 vertical and 4900 oblique UAV images were processed following a multi-image photogrammetric workflow, to produce a digital surface model with a resolution of 1 cm. We then use this data to set up the RoG model and to analyze flood scenarios for various return periods to obtain sub-meter-level hydraulic parameters and evaluate how the site’s vulnerability to flood intrusion might change if its existing wall obstructions were to be extended.

The proposed methodology offers a robust means to extract high-resolution boundary conditions for advanced computational fluid dynamics simulations. Using our multi-scale workflow, relevant stakeholders can enhance their data-driven decision-making for cultural heritage protection and preservation purposes.

Acknowledgments: This work is based on procedures and tasks implemented within the project “Toolbox for assessing and mitigating Climate Change risks and natural hazards threatening cultural heritage—TRIQUETRA”, which is a Project funded by the EU HE research and innovation program under GA No. 101094818.

How to cite: Alexopoulos, M. J., Iliopoulou, T., Istrati, D., Soile, S., Verykokou, S., Ioannidis, C., and Koutsoyiannis, D.: A Multi-Scale Framework for Flood Risk Assessment in Cultural Heritage Sites: The Apollo Temple in Aegina, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18452, https://doi.org/10.5194/egusphere-egu25-18452, 2025.

EGU25-18757 | Orals | CL3.2.7

The GREENART project: "green" and sustainable materials for cultural heritage conservation 

David Chelazzi, Giovanna Poggi, and Piero Baglioni

European Cultural Heritage (CH) is a crucial resource that must be maintained, preserved and made accessible, to counteract degradation enhanced by unfavorable environmental conditions and climate changes. Some of the conservation methodologies nowadays available lack sustainability and cost-effectiveness, and are typically based on energy-consuming processes or non-environmentally friendly materials. This contribution will report on the main results so-far achieved in the EU-funded project GREen ENdeavor in Art ResToration (GREENART), coordinated by the Center for Colloid and Surface Science of the University of Florence (CSGI). Coping with the imperatives of EU Green Deal, the project proposes new solutions based on green and sustainable materials and methods, to preserve, conserve and restore CH. In particular, several innovative materials have been developed and tested:  1) Protective coatings based on green materials from waste and plant proteins, with self-healing and reversibility character, possibly functionalized with organic/inorganic nanoparticles to impart VOC capture, anti-corrosion and barrier behaviors. 2) Foams and packaging materials made by biodegradable/compostable polymers from renewable sources (polyurethanes and natural fibers) to control temperature and relative humidity. 3) Consolidants based on natural polymers from renewable sources, to mechanically strengthen weak artifacts. 4) Gels and cleaning fluids inspired by the most advanced systems currently available to conservators, which will be improved according to green metrics and circular economy requirements. 5) Green tech solutions for monitoring CH assets non-invasively against pollutants and environmental oscillations. Life Cycle Assessment and modeling favor the “safe-by-design” creation of affordable solutions safe to craftspeople, operators and the environment, and minimize energy-consumption in monitoring museum environments. Such holistic approach is granted in GREENART by a multidisciplinary partnership that gathers hard and soft sciences and engineering, including academic centers, innovative industries and SMEs, conservation institutions and professionals, museums whose collections hold absolute masterpieces in need of conservation, public entities and policy makers. Innovative materials and products have been assessed at the lab scale on representative mock-ups of works of art (remedial conservation), or in simulated museum/archive environments (preventive conservation). The project intends to transfer the most promising systems to field assessment on actual artefacts and museums/archives, in cooperation with conservator partners. The best products are also fed into a GREENART open repository and an App to illustrate the new solutions and involve citizens in good preservation practices. Constant feedback from conservators (internal or external to the partnership) can stimulate iterative refinement of the products, triggering a positive loop in this methodological approach. Covering these topics, we provide here an overview of the most advanced green materials for art conservation that can be useful to end-users in this field.

How to cite: Chelazzi, D., Poggi, G., and Baglioni, P.: The GREENART project: "green" and sustainable materials for cultural heritage conservation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18757, https://doi.org/10.5194/egusphere-egu25-18757, 2025.

EGU25-19235 | Posters on site | CL3.2.7

A Smart Decision Support System for the Mitigation of Climate Change Effects on Cultural Heritage 

Vassiliki Charalampopoulou, Anastasia Anastasiou, Efthymios Magkoufis, Konstantinos Mpotonakis, and Christos Kontopoulos

Nowadays Cultural Heritage (CH) monuments face increasing effects of climate change (CC) that vitally impact their sustainability. The TRIQUETRA project, recognising the cruciality of the identification, quantification and mitigation of those CC-driven effects, aims to develop a novel Decision Support System (DSS) that leverages the existing knowledge, to efficiently provide a holistic approach for the conservation of the CH monuments.

More specifically, the TRIQUETRA project focuses on developing a comprehensive, evidence-based DSS for the identification and mitigation of the impacts of climate change on CH sites. TRIQUETRA is based on three key components i.e., Risk Identification, Risk Quantification, and Risk Mitigation. The basis for the DSS is the TRIQUETRA Knowledge Base Platform (KBP), which serves as a dynamic electronic repository equipped with advanced search functionalities and visualisation tools. The KBP concentrates a wide array of validated data regarding a wide variety of CH sites around the world, which climatic, geological and historical records, site-specific attributes, risk assessment, and mitigation strategies are provided through verified research publications.

The DSS features two distinctive modules: the a) Risk Severity Quantification module and b) the Mitigation Measure Selection and Optimisation module. The latter utilises the catalogued information of KBP to provide tailored mitigation measures for each pilot site and verify them based on project outcomes. By incorporating dynamic user stories that consistently reflect the stakeholders' needs, this module facilitates the selection of the most appropriate preservation and mitigation strategies for each site.

Moreover, to enhance functionality, the DSS integrates a search mechanism that allows users to filter results based on a series of criteria such as cost, implementation timeframe, topological effect, etc. The algorithm is adaptable to diverse user inputs and constitutes a scalable solution, leveraging the database of the KBP to identify optimal mitigation solutions, by cross-referencing the characteristics of a given CH site with those of similar sites documented in the relevant literature, providing users with a ranked list of applicable measures.

This adaptive module and the TRIQUETRA DSS as a whole aim to complement research contributing to the protection of cultural heritage against climate change, enabling tailored monitoring and preservation strategies for each pilot CH site.

How to cite: Charalampopoulou, V., Anastasiou, A., Magkoufis, E., Mpotonakis, K., and Kontopoulos, C.: A Smart Decision Support System for the Mitigation of Climate Change Effects on Cultural Heritage, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19235, https://doi.org/10.5194/egusphere-egu25-19235, 2025.

EGU25-19445 | ECS | Posters on site | CL3.2.7

Wave Hazards on Underwater cultural Heritage: The Impact of Climate Change on Cadiz Bay  

Carmen Ferrero Martín, Alfredo Izquierdo, Manuel Bethencourt, Lorenzo Mentaschi, and Tomás Fernández Montblanc

The combination of future Sea level rise and changes in wave climate in coastal areas represents one of the greatest threats to the preservation of underwater cultural heritage (UCH). This study presents a new methodology to assess climate change’s impacts on UCH preservation in shallow waters, focusing on wave-induced hazards like decontextualization of archaeological object, scouring, and wear erosion caused by sediment transport. The approach uses hybrid downscaling of bias-corrected wave fields to assess the changes on this hazard and associated risk under RCP4.5 and RCP8.5 CMIP5 scenarios. The methodology was applied in the Bay of Cadiz, where an overall reduction in wave energy flux was observed. However, local increases were detected in rocky shoals and in the coastal zone, both areas with high UCH density. As a result, the shallow zones exhibited significant changes in decontextualization and scouring hazards. However, the most relevant risk changes were linked to wear erosion, particularly at sites on rocky outcrops near Cadiz. The developed methodology tested in this study is essential for identifying areas with higher risk and for evaluating UCH preservation under future climate conditions. It offers an effective tool for screening sites at risk and for conducting a long-term assessment of these risks in coastal environments affected by climate change.

How to cite: Ferrero Martín, C., Izquierdo, A., Bethencourt, M., Mentaschi, L., and Fernández Montblanc, T.: Wave Hazards on Underwater cultural Heritage: The Impact of Climate Change on Cadiz Bay , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19445, https://doi.org/10.5194/egusphere-egu25-19445, 2025.

EGU25-19751 | ECS | Posters on site | CL3.2.7

CFD investigation of wave runup on coastal cliffs for impact assessment on cultural heritage 

Raouf Sobhani, Denis Istrati, Salvatore Martino, Gian Marco Marmoni, and Federico Feliziani

Wave runup plays a pivotal role in shaping the stability of coastal cliffs, as it generates hydrodynamic pressures that can compromise their structural integrity over time. These cliffs, especially those near cultural heritage (CH) sites, are vital natural structures that indirectly safeguard invaluable assets. Their destabilization, however, poses significant risks, necessitating a comprehensive understanding of the underlying processes that threaten their stability. Despite growing interest in coastal hazard assessments, there remains a paucity of quantitative studies focused on the interplay between wave runup dynamics and the structural characteristics of cliffs. Addressing this gap is essential for improving risk assessment methodologies and developing effective mitigation strategies.

Field measurements conducted in the Horizon Europe project TRIQUETRA revealed that coastal cliffs rarely conform to idealized vertical geometries. Instead, they often exhibit structural irregularities, such as varying inclinations or pre-existing damage like notches, which can exacerbate their exposure to wave-induced pressures. These variations are critical in determining the wave runup and consequently the exposed height of the cliff, which affects its stability. In this study, computational fluid dynamics (CFD) simulations using the Volume of Fluid (VOF) method were employed to model wave-cliff interactions. The analysis focused on the influence of geometric configurations and structural irregularities on the maximum wave runup and the  hydrodynamic pressure distributions, with particular attention to the behavior of steeply inclined cliffs and notched formations. The results demonstrate that wave runup is significantly amplified on near-vertical cliffs, with this effect becoming more pronounced under larger wave conditions. Conversely, notches reduce overall wave runup as their height increases, redistributing hydrodynamic forces along the cliff face and altering the pressure patterns. These findings highlight the intricate relationship between wave dynamics and structural variations, emphasizing the need for site-specific analyses when assessing cliff vulnerabilities.

By advancing the understanding of wave-cliff interactions, this research provides a valuable contribution to coastal hazard studies, offering new insights into the mechanisms driving cliff instability. The outcomes underscore the importance of integrating advanced CFD tools into risk assessments, enabling the design of targeted mitigation strategies to protect coastal regions and preserve the structural integrity of cliffs that play a critical role in safeguarding nearby CH sites.

Acknowledgments: This work is based on procedures and tasks implemented within the project “Toolbox for assessing and mitigating Climate Change risks and natural hazards threatening cultural heritage—TRIQUETRA”, which is a Project funded by the EU HE research and innovation program under GA No. 101094818.

 

 

 

How to cite: Sobhani, R., Istrati, D., Martino, S., Marmoni, G. M., and Feliziani, F.: CFD investigation of wave runup on coastal cliffs for impact assessment on cultural heritage, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19751, https://doi.org/10.5194/egusphere-egu25-19751, 2025.

EGU25-21315 | ECS | Posters on site | CL3.2.7

Aerial and ground-based surveying and 3D modeling of cultural heritage – a case study in Messolonghi, Western Greece 

Panagiotis Tsikas, Aggeliki Kyriou, Epameinondas Lyros, Konstantinos Nikolakopoulos, and Christoforos Pappas

Digital twins of cultural heritage are urgently needed for both comprehensive documentation and digitalization of the monuments, and, also, for the efficient planning of restoration activities towards increased resilience to climatic stressors. Here, we present a workflow for geodetic field surveying followed by 3D building information modeling (BIM), to create a digital twin of an example historical building of Western Greece, the ‘Old Hatzikosta Hospital’ in Messolonghi. More specifically, a detailed point cloud was generated, based on data collected with a Terrestrial Laser Scanner. Building features not directly detectable from the ground (e.g., rooftops) were mapped with photogrammetry using an Unmanned Aerial Vehicle (UAV). The collected data were then further analysed to derive a detailed 3D model of the monument. This 3D model could serve as a baseline for future engineering applications, such as planning maintenance and restoration interventions. Moreover, the digitalization of cultural heritage could also assist in raising public’s awareness and making such historical buildings more widely visible and accessible (e.g., virtual tours, interactive geodatabases etc.).

How to cite: Tsikas, P., Kyriou, A., Lyros, E., Nikolakopoulos, K., and Pappas, C.: Aerial and ground-based surveying and 3D modeling of cultural heritage – a case study in Messolonghi, Western Greece, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21315, https://doi.org/10.5194/egusphere-egu25-21315, 2025.

Integrating High-Performance Computing (HPC) and cloud computing in climate sciences is difficult, due to intricate hardware/software, compatibility, performance and reproducibility issues. Here, we address these challenges in a user-friendly way by leveraging the Conda ecosystem and containers.

Containerization allows to match or exceed native performance on HPC while ensuring bit-for-bit reproducibility for deterministic algorithms and similar processor architectures. This approach simplifies deploying climate models across different platforms; for example, CESM 2.2.2 (Community Earth System Model) provides on various clusters throughputs in simulated years per computational day within +/- 1% of bare-metal performance for simulations spanning thousands of processors.

Exclusively using generic Conda packages for MPI (Message Passing Interface) applications was challenging in HPC. Although OpenMPI included UCX (Universal Communication X) and OFI (Open Fabric Interface), it lacked UCC (Unified Collective Communication) and wasn't optimized by default for high-performance networks like InfiniBand, RoCE (Remote Direct Memory Access over Converged Ethernet) and HPE (Hewlett Packard Enterprise) Slingshot-11, often defaulting to TCP/IP (Transmission Control Protocol/Internet Protocol) or failing. 
 
After updating Conda-Forge’s OpenMPI and MPICH feedstocks, we are adding MVAPICH and ParaStationMPI support to PnetCDF, HDF5, NetCDF-C, NetCDF-Fortran and ESMF (Earth System Modeling Framework) libraries critical for modellers, alongside libFabric and openPMIx (Process Management Interface - Exascale). This incidentally exposed ABI (Application Binary Interface) compatibility issues. Now, MPI toolchains featuring major UCX/OFI/PMIx versions ensure consistent operation across different hosts without affecting numerical results. Using the same Conda environment inside a container, and no hardware-specific optimization, preserves bitwise reproducibility. OMB (Ohio State University Micro-Benchmark) tests for latency, bandwidth and other metrics help confirm if optimal performance can be achieved or not. 

Such developments enable climate scientists to focus on addressing scientific questions rather than sorting out software dependencies and technical problems. One can write code on a laptop then effortlessly scale to cloud or supercomputers, and seamlessly run climate simulations somewhere then continue these wherever compute resources are available without worrying about discontinuities. This also releases expensive HPC resources for production instead of wasting them for training, learning, development or testing which can be performed comfortably elsewhere, without job scheduling constraints, in the very same software environment.

Conda has primarily been developed with a focus on compatibility which limits its suitability in highly performance-sensitive applications where locally optimized builds of specific key components are paramount, typically in climate modeling. Additionally, instead of relying on local engineers to install and maintain host software, Conda users can benefit from the work of thousands of open-source contributors who continuously update and test the entire ecosystem.

This strategy fits the session's theme by providing a framework where cloud resources can be utilized for big data without compromising the performance or rigor of HPC environments. Conda and container technologies ought to change how climate scientists approach software management, focusing on ease of use, scalability and reproducibility, thereby potentially altering practices within the field to improve usage of computational resources and leverage community efforts to remain at the forefront.

How to cite: Iaquinta, J., Fouilloux, A., and Ragan-Kelley, B.: Climate Modeling with Conda and Containers to Improve Computational Resource Usage while Achieving Native Performance and Reproducibility, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2605, https://doi.org/10.5194/egusphere-egu25-2605, 2025.

EGU25-6798 | Orals | ESSI2.15

Advancing Geophysical Data Analysis: HEALML for Efficient Sphere-Based Statistics on Pangeo-EOSC 

Jean-Marc Delouis, Erwan Allys, Justus Mangin, Louise Mousset, and Tina Odaka

A significant challenge in data integration and ML methodologies on cloud infrastructures is accurately determining correlated statistics. Initially, aligning data to a consistent pixel grid is essential, motivating the use of Discrete Global Grid Systems (DGGS). In geophysical studies, data reside on a sphere, and approximating with tangent planes can distort results. Our solution is the HEALPix pixelization as our DGGS framework, standardizing data on a common grid for consistent statistical analysis. HEALPix's unique features, such as its iso-latitude layout and uniform pixel areas, enable the use of spin-weighted spherical harmonics in managing vector fields. This enables the accurate calculation of  correlation statistics, such as between velocity and scalar fields on the sphere, while minimizing biases due to spherical approximations. By utilizing the HEALPix framework, known in cosmology, with TensorFlow or PyTorch as backends, we created the: HEALML library. This library facilitates gradient computations of all derived statistics for AI optimization, and has been validated on the Pangeo-EOSC platform. This library parallelizes the computation of localized spherical harmonics and includes features like scattering covariance calculations, allowing the extraction of more complex nonlinear statistics beyond the power spectrum. We compare these results to traditional 2D planar methods, demonstrating the advantages of sphere-based statistics on platforms like Pangeo-EOSC. Furthermore, we demonstrate: HEALML's ability to emulate using a substantially smaller dataset. This demonstration emphasizes the ways in which incorporating spherical statistical methods into Pangeo-EOSC fosters innovative and efficient statistical analysis within geophysical research.

How to cite: Delouis, J.-M., Allys, E., Mangin, J., Mousset, L., and Odaka, T.: Advancing Geophysical Data Analysis: HEALML for Efficient Sphere-Based Statistics on Pangeo-EOSC, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6798, https://doi.org/10.5194/egusphere-egu25-6798, 2025.

EGU25-8127 | ECS | Posters on site | ESSI2.15

Seamless Upscaling Research from Cloud to HPC using eWaterCycle 

Mark Melotto, Rolf Hut, and Bart Schilperoort

The eWaterCycle platform provides hydrologists with a platform that allows them to work with each other's models and data without having to become a computer scientist in the process. The eWaterCycle platform supports existing hydrological models and makes them available for scientists using the BMI model interface as a communication layer. Models run in containers for reproducibility and dependency control. Popular hydrological models are readily available (PCRGLobWB, WFLOW, HBV, etc.). Scientists develop their analyses or experiments in the widely known JupyterHub environment. 

While in theory eWaterCycle can be installed and run on any hardware, in practice most users interact with it on the SURF Research Cloud, a cloud computing infrastructure available to the Dutch academic ecosystem. Until recently upscaling from Cloud to HPC infrastructure for larger model runs required extensive knowledge of the HPC system. Here we will present our work on building a seamless workflow that allows scientists to upscale their cloud based work to the Snellius supercomputer and the Spider grid computer without having to worry about technical issues like mounting points for (large) datasets and container engines.

Our workflow opens up the possibility for more scientists to benefit from HPC and Grid resources while focussing on their domain science. We present the workflow in such a format that it should be easily portable to other hybrid cloud - HPC infrastructures, including the DestinE systems.

How to cite: Melotto, M., Hut, R., and Schilperoort, B.: Seamless Upscaling Research from Cloud to HPC using eWaterCycle, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8127, https://doi.org/10.5194/egusphere-egu25-8127, 2025.

We present recent progress around the EERIE cloud data server (https://eerie.cloud.dkrz.de) and its software stack “cloudify”. The EERIE cloud provides efficient open access to prominent climate datasets stored on disk at the German Climate Computing Center (DKRZ).

A new kerchunk-plugin enables data access to raw model output as-is to enable verifiable data transfer with better latency. STAC (Spatio Temporal Assets Catalog) catalogs are deployed and displayed through the EERIE cloud to make the provided DKRZ datasets findable and accessible. Two in-browser apps can be started, pre-configured for each dataset, by just clicking buttons: (1) the data visualization app “gridlook” as well as a (2) jupyterlite for interactive analysis and monitoring. 

We leverage the python package xpublish, a plugin for Pangeo's central analysis package Xarray. Its main feature is to provide ESM output by mapping any input data to virtual zarr datasets. Users can retrieve these datasets as if they were cloud-native and cloud-optimized.

How to cite: Wachsmann, F.: The EERIE cloud: Apps and Catalogs for Cloudified Earth System Model Output, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8591, https://doi.org/10.5194/egusphere-egu25-8591, 2025.

EGU25-8754 | ECS | Orals | ESSI2.15

Leveraging Cloud, Earth Observation and In-Situ Sensors for Agri-Environmental Monitoring and Policy Decision-Making  

Georgios Charvalis, Panagiota Louka, Vassileios Gkoles,  Thanasis Manos, Nikos Kalatzis, Dionysios Solomos, Anastasios Trypitsidis, and Odysseas Sekkas

Cloud infrastructures play a significant role in delivering secure, scalable and efficient data processing for Earth Observation (EO) and agricultural management applications. As part of the ScaleAgData project, we present a hierarchical Agri-Environmental Monitoring Tool running on a private cloud infrastructure. The system combines data from EO, in-situ sensors and farm management information systems (FMIS), including parcel calendars, to provide farmers and policymakers multi-scale insights.  

The solution is cloud-based and designed with an underlying architecture that ensures both scalability and interoperability, leveraging OGC-compliant data formats where applicable. EO and in-situ data streams can be processed and analyzed efficiently with the help of containerized apps and microservices to facilitate modular development and simplify deployment. By using a web-based dashboard with hierarchical design, stakeholders can navigate from overviews at the municipal level to individual parcels. Aggregated summaries that comply with Common Agricultural Policy (CAP) criteria are useful to policymakers and farmers can get comprehensive parcel-level metrics to optimize irrigation, pesticide use and other agro-related activities.  

Specifically, the tool combines EO data to derive vegetation indices (e.g., NDVI, EVI) and other parameters requiring advanced processing for crop type classification. Furthermore, these datasets are enriched with in-situ sensor measurements (e.g. soil moisture, weather data) and farm logs managed within FMIS (irrigation schedule, pesticide usage). Parcel-level data (L1) is processed to generate statistics, which are then calibrated with nearby parcels data with similar properties and crop type(L2), serving as control level, and finally extrapolated to the municipal level (L3) using spatial averaging techniques  to provide indicators related to irrigation water, pesticide, fertilizer usage, etc.  Farm calendars stored within FMIS provide a reliable source of ground-truth data, enhancing the tool’s ability to validate aggregated metrics. The aggregation at L2 and L3 allows for the identification of regional trends and patterns in agricultural practices, empowering policymakers and stakeholders to implement targeted interventions at both levels, thereby promoting sustainable agriculture.   

This work showcases the potential of private cloud infrastructures to enhance agri-environmental monitoring by processing and integrating heterogeneous data streams (EO, in-situ sensors and farm log data) into a unified system. The system is being applied in diverse agricultural regions of Greece (Crete, Thessaly, Macedonia) with ongoing validation efforts aimed at refining its accuracy and adaptability. Future work includes the integration of cloud-based machine learning models and EO-derived evapotranspiration data to enhance the efficiency of extrapolating parcel-level (L1) and regional (L2) metrics into policy-level indicators (L3). Additionally, alternative aggregation methods, such as model-based approaches, spatial regression, and interpolation techniques like Kriging, will be tested to improve the accuracy and reliability of aggregated insights. 

How to cite: Charvalis, G., Louka, P., Gkoles, V., Manos,  ., Kalatzis, N., Solomos, D., Trypitsidis, A., and Sekkas, O.: Leveraging Cloud, Earth Observation and In-Situ Sensors for Agri-Environmental Monitoring and Policy Decision-Making , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8754, https://doi.org/10.5194/egusphere-egu25-8754, 2025.

EGU25-9432 | Posters on site | ESSI2.15

Co-Creating Cloud-Based Tools for Urban Climate-Resilience: The CLIMRES Project 

Claudio Pisa, Marica Antonacci, Vasileios Baousis, Sotirios Aspragkathos, Iasonas Sotiropoulos, and Stamatia Rizou

Europe faces a growing frequency of extreme weather events, from heatwaves and floods to wildfires and earthquakes, increasingly threatening urban environments. Unusually warm winters are becoming progressively common, destabilizing ecosystems and altering traditional weather dynamics. 

Addressing these crucial changes, the CLIMRES project aims to foster a “Leadership for Climate-Resilient Buildings” by identifying and categorizing vulnerabilities within the built environment and assessing their effects within urban systems. This effort integrates diverse data sources, including Copernicus services, IoT networks, and municipal datasets, and considers hazard warnings and weather forecasts. Moreover, a liaison with the Destination Earth initiative enhances the project with the capacity to leverage extreme weather predictions and future climate models. 

CLIMRES aims to deliver vulnerability assessment and impact evaluation methodologies, along with a “hub of measures” inventory for cost-effective building design and materials against climate risks, as well as decision support tools, to aid building owners, policymakers and stakeholders in planning effective interventions and to address vulnerabilities, targeting three levels of decision making at strategic, tactical and operational levels. The project deploys cloud technologies like OpenStack and Kubernetes to host an interoperable platform for vulnerability analysis, data harmonization, and decision-making. Its solutions will be tested and validated on 3 Large Scale Pilots in Spain, Greece, Italy, and Slovenia, addressing hazards such as heatwaves, flooding, fires, and earthquakes. A multi-hazard replication pilot in France will further evaluate the scalability and versatility of these approaches across diverse contexts. 

Insights from these pilots will feed into a replication roadmap and a capacity-building program designed to train future leaders in climate-resilient urban development. By fostering co-creation with local stakeholders and communities, CLIMRES ensures its innovative solutions are practical, cost-effective, and replicable, targeting Technology Readiness Levels (TRL) 6-8. 

CLIMRES aims to bridge innovation with actionable solutions, equipping building owners, policymakers, and communities with the tools needed to enhance urban climate resilience. This presentation highlights the project’s interdisciplinary approach, outputs and technological underpinnings, offering insights into scalable solutions for climate adaptation in urban settings. 

How to cite: Pisa, C., Antonacci, M., Baousis, V., Aspragkathos, S., Sotiropoulos, I., and Rizou, S.: Co-Creating Cloud-Based Tools for Urban Climate-Resilience: The CLIMRES Project, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9432, https://doi.org/10.5194/egusphere-egu25-9432, 2025.

EGU25-10683 | Orals | ESSI2.15

Copernicus data and services uptake with EO4EU platform: an AI-augmented ecosystem for Earth Observation data accessibility and exploitation. 

Federico Fornari, Vasileios Baousis, Mohanad Albughdadi, Marica Antonacci, Tolga Kaprol, Claudio Pisa, Charalampos Andreou, Kakia Panagidi, and Stathes Hadjiefthymiades

The Copernicus program has fostered Earth Observation (EO) and Earth Modeling by offering extensive data and services to European Citizens. Sentinel satellites’ data is accessible  through platforms like the Copernicus Open Access Hub and the Copernicus Data Space Ecosystem, which provide a wide range of information on land, ocean and atmospheric conditions. Complementing these resources, six specialized Copernicus services deliver data in domains such as the atmosphere, marine environment, land monitoring, climate change, security and emergency response. To streamline access and usability, cloud-based Copernicus Data and Information Access Services (DIAS) offer centralised platforms equipped with cloud infrastructure and processing tools. Building on these efforts, the Copernicus Data Space Ecosystem (https://dataspace.copernicus.eu/) enhances existing DIAS services with advanced functionalities like improved search capabilities, virtualizations and APIs. Meanwhile, the Destination Earth (DestinE) initiative led by ECMWF, EUMETSAT and ESA, aims to develop high-precision digital Earth models - or digital twins - that simulate natural and human activities. These models mainly focus on weather-induced extremes and climate change adaptation, generating valuable Earth Modeling data. Furthermore, European Data Spaces integrate datasets across diverse domains, including agriculture, health, energy, and environmental monitoring, creating opportunities to combine these resources with Copernicus and DestinE data through advanced technologies like artificial intelligence (AI) and machine learning (ML). This integration paves the way for innovative solutions and public-facing products and services. Despite the volume and richness of Copernicus and related EO data, its accessibility remains limited, with most users being experts or scientists. For broader industry adoption and the development of impactful applications that benefit society and the enviroment, significant barriers must be addressed. EO data is often fragmented, complex, and difficult to process, requiring domain expertise for tasks such as data discovery, pre-processing, storage, and conversion into formats suitable for analytics and Geographic Information Systems (GIS).

The EO4EU platform (https://www.eo4eu.eu/), showcased in this presentation, introduces a multi-cloud ecosystem designed for holistic management of EO data. Its primary objective is to bridge the gap between domain experts and end users, leveraging technological advancements to broaden the adoption of EO data across diverse markets. By enhancing the accessibility and usability of EO data, EO4EU supports market growth through advanced data modeling, dynamic annotation, and state-of-the-art processing, powered by European cloud infrastructures such as WEkEO/DIAS and CINECA. EO4EU provides a suite of innovative tools and methodologies to assist a wide range of users, from professionals and domain experts to general citizens, in benefiting from EO data. Its key features include:

  • Knowledge Graph-based Decision Making: Facilitates insightful feature extraction from diverse repositories, enabling a more comprehensive understanding of datasets.
  • AI/ML Marketplace: A centralized hub for AI & ML models, algorithms, techniques, and metadata.
  • Big Data Processing Engines: Optimized for cloud environments to efficiently manage large-scale datasets.
  • User-friendly Interfaces: GUI, CLI, APIs, and immersive VR experiences, targeting both technical and non-technical users.
  • Workflow Engine: Simplifies the definition and execution of recurring tasks for EO data retrieval and processing.

How to cite: Fornari, F., Baousis, V., Albughdadi, M., Antonacci, M., Kaprol, T., Pisa, C., Andreou, C., Panagidi, K., and Hadjiefthymiades, S.: Copernicus data and services uptake with EO4EU platform: an AI-augmented ecosystem for Earth Observation data accessibility and exploitation., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10683, https://doi.org/10.5194/egusphere-egu25-10683, 2025.

EGU25-10977 | Posters on site | ESSI2.15

Cloud-Powered Earth Observation Tools for Urban Resilience: The BUILDSPACE Project 

Marica Antonacci, Vasileios Baousis, Claudio Pisa, Stamatia Rizou, and Iasonas Sotiropoulos

The BUILDSPACE project harnesses the transformative potential of cloud computing to evolve urban development and resilience practices. By integrating advanced Earth Observation (EO) data with state-of-the-art satellite and cloud technologies, BUILDSPACE addresses critical urban challenges, including climate adaptation, energy efficiency, and disaster resilience, while contributing to the European Green Deal’s objectives of sustainability and carbon neutrality. 

Central to BUILDSPACE are five innovative services designed to support urban decision-making. At the building scale, the project facilitates the generation and visualization of detailed digital twins through interactive displays, virtual reality (VR), and augmented reality (AR) interfaces. These digital twins enable precise simulations for energy optimization, operational efficiency, and climate impact assessment. At the city scale, BUILDSPACE provides tools to address climate scenarios, such as urban heat islands and flooding, empowering municipalities and urban planners with actionable insights through interactive, map-based platforms. 

The project’s technical foundation lies in a robust, cloud-native architecture built on Kubernetes and OpenStack, combined with a DevOps methodology to streamline both infrastructure services and application deployment. Kubernetes orchestrates containerised workloads, enabling efficient automated deployment, scaling and management of applications, while OpenStack provides a flexible infrastructure for managing compute, storage, and networking resources. Through the DevOps approach, we ensure continuous integration and delivery (CI/CD), fostering rapid development cycles and operational agility. By adopting open-source cloud platforms, the project ensures interoperability, reproducibility and automation across diverse environments, driving consistency and efficiency throughout the lifecycle of both infrastructure and applications. 

The project’s services are being validated across four European cities representing diverse climatic conditions, namely Warsaw, Riga, Piraeus and Ljubljana. These validations focus on two scenarios: construction companies monitoring building processes with advanced digital tools, and municipalities analysing the impacts of climate change on urban infrastructure. 

By advancing from TRL 5-6 to TRL 7-8, BUILDSPACE aims to deliver market-ready solutions that align with the European GNSS and Copernicus initiatives and to synchronise with the advances, concerning Digital Twin technologies and data federation mechanisms, of the Destination Earth initiative, while paving the way for a broader adoption of cloud technologies in EO-based urban resilience applications. 

How to cite: Antonacci, M., Baousis, V., Pisa, C., Rizou, S., and Sotiropoulos, I.: Cloud-Powered Earth Observation Tools for Urban Resilience: The BUILDSPACE Project, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10977, https://doi.org/10.5194/egusphere-egu25-10977, 2025.

EGU25-11810 | Orals | ESSI2.15

DeployAI Earth Observation Services: Enabling Environmental Insights on the European AI-on-Demand Platform 

Antonis Troumpoukis, Mohanad Albughdadi, Martin Welß, Vasileios Baousis, and Iraklis Klampanos

The DeployAI project [1] designs and delivers a fully operational European AI-on-Demand Platform (AIoDP) to empower the European industry with access to cutting-edge AI technology, and to promote trustworthy, ethical, and transparent European AI solutions, with a focus on SMEs and the public sector. To achieve this, the platform enables the development and deployment of AI solutions through the following core solutions: (i) AI Builder [2], which allows the assembling of reusable AI modules into AI pipelines; (ii) seamless access to Cloud and HPC infrastructures (e.g., MeluXina and LUMI); (iii) a marketplace for the listing and distribution of ready-to-use AI products; (iv) an expansive and growing library of diverse AI-driven use cases.

As part of its domain-driven solutions, AIoDP seeks to empower Environmental Scientists, AI Engineers, Developers, Researchers, and SMEs via the DeployAI Earth Observation Services. These services will accelerate the development of AI-driven environmental applications, by providing pre-trained models that simplify satellite imagery processing, land usage classification, and image segmentation. Key models available as modules within the DeployAI’s AI Builder include:

  • Leaf Area Index (LAI) Model: Enables precise monitoring of vegetation health and ecological dynamics by calculating leaf area per unit ground [3]. 
  • Object Detection Model: Identifies specific objects in high-resolution satellite images, supporting applications such as  infrastructure monitoring, pollution tracking, and deforestation assessment [4].
  • Segment Anything Model (SAM): Simplifies analysis across diverse environmental applications through the capabilities of SAM that allows flexible, prompt-based image segmentation for new datasets, with zero-shot and few-shot learning [5].

These models, along with the broader functionalities of AI Builder, enable users to create custom AI pipelines that address their specific environmental challenges in several environmental areas, including vegetation health monitoring, water balance analysis, climate modeling, urban planning, traffic management, pollution monitoring, and infrastructure maintenance. Users can leverage the visual pipeline editor to easily assemble pipelines from reusable AI modules without needing to write code. Once created, these pipelines can be deployed as AI applications on various execution environments. DeployAI facilitates seamless transitions between these environments by providing connectors to a host of target infrastructures, including Cloud platforms and HPC systems. This empowers users to leverage the most suitable computational resources for their specific needs.

By providing a user-friendly platform with access to cutting-edge AI technology and Cloud/HPC resources, DeployAI empowers users to address critical environmental challenges and unlock new possibilities for sustainable development.

[1] https://deployaiproject.eu
[2] https://gitlab.eclipse.org/eclipse/graphene
[3] https://github.com/DeployAI-Environmental-Services/depai-lai
[4] https://github.com/DeployAI-Environmental-Services/depai-yolov8-obb
[5] https://github.com/DeployAI-Environmental-Services/depai-sam-interactive

This work has received funding from the European Union’s Digital Europe Programme (DIGITAL) under grant agreement No 101146490.

How to cite: Troumpoukis, A., Albughdadi, M., Welß, M., Baousis, V., and Klampanos, I.: DeployAI Earth Observation Services: Enabling Environmental Insights on the European AI-on-Demand Platform, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11810, https://doi.org/10.5194/egusphere-egu25-11810, 2025.

EGU25-12070 | ECS | Orals | ESSI2.15

Performance Benchmarking and Energy monitoring for Climate Modelling 

Sergi Palomas, Mario Acosta, Gladys Utrera, Okke Lennart, Daniel Beltran, Miguel Castrillo, Niclas Schroeter, and Ralf Mueller

The computational intensity of climate models makes them among the most energy-demanding applications in High-Performance Computing (HPC), resulting in significant computational costs and carbon emissions. Addressing the dual challenge of improving climate predictions —by running higher resolution, more accurate and complex models— and ensuring sustainability requires innovative tools to evaluate both computational efficiency and energy consumption across diverse HPC architectures. To address this, and in the context of the Center of Excellence in Simulation of Weather and Climate in Europe (ESiWACE), we have extended the High-Performance Climate and Weather Benchmark (HPCW) framework to incorporate a standardised set of Climate Performance Metrics for Intercomparison Projects (CPMIPs) and energy consumption monitoring.

HPCW, originally designed to maintain a set of relevant and realistic, near-operational weather forecast workloads to benchmark HPC sites, can provide insights beyond generic benchmarks like High-Performance Linpack (HPL) or High-Performance Conjugate Gradients (HPCG) by focusing on domain-specific workloads.

The inclusion of CPMIPs into HPCW brings a widely accepted set of metrics specifically tailored to the particularities of climate workflows. These metrics, already recognized by the scientific community, are key to better understanding climate model performance and allow us to keep the results from the framework relevant for research and operational runs, as well as improving our capacity for multi-model multi-platform performance comparisons.

By integrating energy monitoring, HPCW enables users to evaluate how critical computational kernels in climate models perform in terms of energy consumption. Our review of energy profiling tools across EuroHPC pre-exascale systems, including MareNostrum 5, LUMI, and Leonardo, highlights a fragmented landscape. Current tools offer varying granularity and portability, but limitations such as system configurations, administrative restrictions, and hardware compatibility often hinder their application. Low-level interfaces like Running Average Power Limit (RAPL) and Performance Application Programming Interface (PAPI) counters offer precise energy measurements but are constrained by accessibility issues.

These advancements aim to improve the allocation of climate experiments, such as those conducted for the Intergovernmental Panel on Climate Change (IPCC) in Coupled Model Intercomparison Projects (CMIPs), to the most suitable HPC resources, while also identifying architectural bottlenecks before running production experiments. Additionally, by enhancing energy consumption quantification, this work contributes to ongoing efforts to measure and reduce the carbon footprint of the climate research community. Furthermore, these analyses are expected to be particularly valuable for climate researchers, especially in the context of upcoming large-scale initiatives like CMIP7, enabling them to make informed resource requests and facilitate robust multi-platform comparisons of climate model performance which were not possible in the past. We anticipate that HPC vendors can also benefit from the outcomes of our work in optimising the systems for climate modelling workloads. By combining performance and energy metrics within a unified framework, we provide critical insights that align computational advancements with sustainability goals, ensuring efficient and environmentally conscious use of HPC resources for climate research.

How to cite: Palomas, S., Acosta, M., Utrera, G., Lennart, O., Beltran, D., Castrillo, M., Schroeter, N., and Mueller, R.: Performance Benchmarking and Energy monitoring for Climate Modelling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12070, https://doi.org/10.5194/egusphere-egu25-12070, 2025.

EGU25-12918 | ECS | Orals | ESSI2.15

Enhancing Pangeo-Fish with HEALPix Convolution: Impact Evaluation and Benefits 

Etienne Cap, Tina Odaka, Jean-Marc Delouis, Justus Magin, and Mathieu Woillez

The Pangeo-Fish project processes biologging data to analyze fish movement and migration patterns.  While SciPy’s convolution methods are robust, they are not optimized for handling spherical datasets inherent to Earth system science. To address this limitation, we propose the integration of HEALPix convolution, a method designed for spherical operations, into Pangeo-Fish.

HEALPix convolution offers distinct advantages for geophysical data analysis, particularly when dealing with spherical datasets in Earth system science. It uses the HEALPix pixelization as a core Discrete Global Grid System (DGGS), which ensures equally-sized pixels globally, removing distortions common in flat projections. This consistency is crucial for maintaining the physical relevance of convolutions across locations. Additionally, HEALPix’s dyadic property supports flexible, multiscale resolution adjustments, allowing for downscaling while preserving accuracy. Such scalability is essential for studying oceanic environments where areas of interest, like coastal zones and basins, are often resolution-dependent.

Our approach evaluates the performance of HEALPix convolution in comparison to traditional SciPy methods, focusing on its ability to enhance the accuracy of habitat mapping and migration pathway modeling for fish. 

This integration is particularly relevant within the Global Fish Tracking System (GFTS), which operates under the European Union’s Destination Earth (DestinE) initiative. GFTS utilizes datasets from Copernicus Marine Services and the European Tracking Network (ETN) to model fish habitats, spawning grounds, and migration swimways. HEALPix convolution strengthens the pangeo-fish’s capacity for studying Species such as tuna and eel that exhibit large-scale, transoceanic migrations.    

In conclusion, this work highlights the transformative potential of HEALPix convolution in spherical data processing. By integrating this innovative method, Pangeo-Fish can provide more accurate, scalable, and actionable insights into fish behaviors and habitats, contributing to sustainable management practices and conservation strategies globally.

 

How to cite: Cap, E., Odaka, T., Delouis, J.-M., Magin, J., and Woillez, M.: Enhancing Pangeo-Fish with HEALPix Convolution: Impact Evaluation and Benefits, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12918, https://doi.org/10.5194/egusphere-egu25-12918, 2025.

EGU25-13725 | Posters on site | ESSI2.15

Cloud-based platform for the management of hydrogeological risks in the Po Basin  

Marco Zazzeri and the PARACELSO team

In recent years, technological advances in the use of geospatial data (such as satellite images, anthropogenic and/or environmental raster and vector open data, etc.) for hydrogeological risk assessment, combined with advanced analysis techniques (e.g., machine learning), have become increasingly valuable. These technologies can be utilized by local and national authorities for land planning and emergency management to better understand the dynamics associated with climate change. This understanding can help guide actions aimed at safeguarding not only environmental resources but also socio-economic assets and citizens’ lives.

In pursuit of this goal, a partnership has been established between the Po River Basin District Authority (AdBPo), the Italian Space Agency (ASI), and academic and research institutions such as the University of Bologna (UNIBO), the University of Modena and Reggio Emilia (UNIMORE), the University of Padova (UNIPD), and the Institute of Environmental Geology and Geoengineering of the National Research Council of Italy (CNR-IGAG). The aim is to implement a downstream service for monitoring landscape evolution related to fluvial systems (geomorphological classification), and slope dynamics (including landslides and rock glaciers) and to quantitatively evaluate the exposed assets.

The PARACELSO project (Predictive Analysis, MonitoRing, and mAnagement of Climate change Effects Leveraging Satellite Observations) aims to develop a modular and interoperable cloud-based platform that supports the analysis of natural phenomena (such as fluvial hydrodynamics, landslides, and rock glaciers) using satellite images provided by:

  • DIAS platforms deployed by the Copernicus Programme (e.g., Sentinel 1-2);
  • ASI missions such as CosmoSkyMed, PRISMA, and SAOCOM.

Furthermore, a methodology integrating Earth Observation and geospatial data analysis has been implemented using open-source libraries.

To facilitate this, the MarghERita supercomputer, named in honor of the scientist Margherita Hack, has been made available by the Emilia-Romagna region. It is used both to store the downloaded satellite images and to run the algorithms developed in the project for studying the temporal evolution of river and slope systems. Finally, it enables the sharing and visualization of processed data.

The project has received funding from ASI through the “I4DP_PA (Innovation for Downstream Preparation for Public Administrations)” Call for Ideas.

How to cite: Zazzeri, M. and the PARACELSO team: Cloud-based platform for the management of hydrogeological risks in the Po Basin , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13725, https://doi.org/10.5194/egusphere-egu25-13725, 2025.

EGU25-13873 | Orals | ESSI2.15

UXarray: Extending Xarray for Enhanced Support of Unstructured Grids 

John Clyne, Hongyu Chen, Philip Chmielowiec, Orhan Eroglu, Cecile Hannay, Robert Jacob, Rajeev Jain, Brian Medeiros, Paul Ullrich, and Colin Zarzycki

Over the past decade, weather and climate models have rapidly adopted unstructured meshes to better leverage high-performance computing systems and approach kilometer-scale resolutions. Output from this new generation of models presents many challenges for their subsequent analysis, largely due to a lack of community tools supporting unstructured grid data. Last year, we introduced UXarray, a class extension of Xarray that provides native support for unstructured meshes. UXarray readily runs in a Jupyter Notebook and offers parallelized execution through its compatibility with Dask, demonstrating its flexibility as both a tool for lightweight exploration and communication, and for supporting intensive calculations applied to vast data volumes. Over the past year, UXarray has matured significantly and is now capable of supporting many real-world analysis workflows applied to outputs from a growing number of high-resolution models and dynamical cores, including ICOsahedral Non-hydrostatic (ICON) atmosphere model, the Finite-Element/volumE Sea ice-Ocean Model (FESOM), NSF NCAR’s Model for Prediction Across Scales (MPAS), and the U.S. DOE’s Energy Exascale Earth System Model (E3SM). This presentation will provide an overview of the UXarray’s current capabilities, which include extensive support for plotting and many foundational analysis operators; demonstrate examples in Jupyter Notebooks; present plans for the future;  and discuss ways for Pangeo and the broader earth system science community to help guide new developments. 

How to cite: Clyne, J., Chen, H., Chmielowiec, P., Eroglu, O., Hannay, C., Jacob, R., Jain, R., Medeiros, B., Ullrich, P., and Zarzycki, C.: UXarray: Extending Xarray for Enhanced Support of Unstructured Grids, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13873, https://doi.org/10.5194/egusphere-egu25-13873, 2025.

EGU25-14306 | ECS | Orals | ESSI2.15

Navigating New Grids: Evaluating DGGS Configurations for Marine Spatial Analysis 

Kayziel Martinez, Alexander Kmoch, Lőrinc Mészáros, Andrew Nelson, and Evelyn Uuemaa

Accurate and efficient spatial analysis is crucial for the mapping and sustainable management of marine environments, where large-scale and diverse datasets present significant analytical challenges. Traditional latitude-longitude methods, while widely used, often encounter limitations in data integration and handling distortion caused by Earth’s curvature. Discrete Global Grid Systems (DGGS) have emerged as a promising solution, offering a hierarchical, global, and equal-area framework for geospatial analysis. Despite their potential, the performance in marine spatial analysis remains underexplored.

This study evaluates the impact and suitability of DGGS-based spatial analysis by comparing its performance with the traditional latitude-longitude approaches. Using marine datasets representing point and raster data formats, the workflow begins with quantization, converting the data into DGGS cells.The implementation utilizes open-source Python tools from the Pangeo ecosystem, including xarray-xdggrid, to enable seamless integration and efficient analysis of large geospatial datasets. Three DGGS configurations – ISEA7H, HEALPIX, and ISEA3H are compared alongside traditional latitude-longitude grid for computational efficiency (processing time and memory usage) and their ability to preserve spatial patterns. Spatial analysis methods include density estimation, nearest neighbor evaluation, and clustering for point data, as well as zonal statistics, spatial autocorrelation, and resampling for raster data.

To further illustrate the application of DGGS-based methods, the study includes a case study on estuary characterization. This characterization relies on spatial analysis methods, integrating physical oceanographic parameters from Delft3D-FM, biogeochemical and optical data products, and in-situ point measurements from the Copernicus Marine Environment Monitoring Service (CMEMS). Representing these diverse datasets within the DGGS framework highlights its ability to manage varying data types and scales, offering insights into estuarine environments and demonstrating its scalability for addressing complex marine spatial challenges.

Results indicate that DGGS frameworks deliver comparable computational performance while offering consistent spatial representation. Configuration-specific trade-offs influence their effectiveness, emphasizing the importance of aligning DGGS configurations with specific analytical tasks and applications. Findings suggest that DGGS-based methods offer a promising alternative to traditional analysis techniques, providing greater flexibility in adapting to datasets, scale, and resolution. This contributes to more efficient mapping, sustainable marine environmental management, and advancing geospatial applications through open-source tools from the Pangeo ecosystem.

How to cite: Martinez, K., Kmoch, A., Mészáros, L., Nelson, A., and Uuemaa, E.: Navigating New Grids: Evaluating DGGS Configurations for Marine Spatial Analysis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14306, https://doi.org/10.5194/egusphere-egu25-14306, 2025.

EGU25-14400 | ECS | Orals | ESSI2.15

A community oriented approach to enabling open science with Earth science data at scale 

Max Jones, Aimee Barciauskas, Jonas Sølvsteen, Brian Freitag, Yuvi Panda, Kyle Barron, Julia Signell, Alex Mandel, Chuck Daniels, Nathan Zimmerman, Sean Harkins, Henry Rodman, Zac Deziel, Slesa Adhikari, Anthony Boyd, Alexandra Kirk, David Bitner, and Vincent Sarago

To enable wider participation in open science with geospatial data at scale, we need to reduce the effort and custom approaches required for setting up scalable scientific data analysis environments and computing workflows. We have made great strides in this pursuit by evolving and promoting community-developed open source frameworks, tools, and libraries for cloud-native data access and analysis, making them the default for scientists on the public cloud and local systems.

Many of our achievements have been supported by the NASA Visualization, Exploration, and Data Analysis (VEDA) project which seeks to proliferate cloud-native approaches for open science on Earth science data from NASA’s rich archives and many other providers. Our presentation highlights how we have engaged with communities like Pangeo, OpenScapes, Earth Science Information Partners, and the Cloud Native Geospatial Forum to build joint initiatives, target development, and ensure uptake of new solutions. We present key results from working groups, community showcases, and hackdays and hackweeks organized by VEDA team members, as well as specific contributions to the open source ecosystem, including the eoAPI platform for quickly and easily deploying an open-source Earth Observation stack, JupyterHub fancy profiles (with BinderHub) for seamless environment building, and Lonboard for fast, interactive vector visualization.

How to cite: Jones, M., Barciauskas, A., Sølvsteen, J., Freitag, B., Panda, Y., Barron, K., Signell, J., Mandel, A., Daniels, C., Zimmerman, N., Harkins, S., Rodman, H., Deziel, Z., Adhikari, S., Boyd, A., Kirk, A., Bitner, D., and Sarago, V.: A community oriented approach to enabling open science with Earth science data at scale, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14400, https://doi.org/10.5194/egusphere-egu25-14400, 2025.

EGU25-14610 | Orals | ESSI2.15

Weather Data Streaming with Kerchunk: Strengthening Early Warning Systems  

Nishadh Kalladath, Masilin Gudoshava, Shruti Nath, Jason Kinyua, Fenwick Cooper, Hannah Kimani, David Koros, Christine Maswi, Zacharia Mwai, Asaminew Teshome, Samrawit Abebe, Isaac Obai, Jesse Mason, Ahmed Amdihun, and Tim Palmer

The Ensemble Prediction System (EPS) provided by global weather forecast centres generates vast amounts of data that is crucial for early warnings of extreme weather and climate. However, regional and national meteorological services often face challenges in processing this data efficiently, particularly during regional downscaling and post-processing. Conventional methods of downloading and storing GRIB-format data have become increasingly inefficient and unsustainable. The Strengthening Early Warning Systems for Anticipatory Actions (SEWAA) project aims to address these challenges by exploring the use of cloud native operations and GenAI-cGAN driven post-processing systems.   

Kerchunk provides a groundbreaking solution for real-time weather data streaming, catering to the transition towards open and free to use cloud-based object storage from global weather forecasting centres. Kerchunk, in conjunction with GRIB index files, enables efficient, real-time access to weather data, fostering more sustainable workflows in weather and climate services, thus strengthening early warning systems.  

This study developed a workflow for streaming forecast data using Kerchunk with two primary objectives:  

1. Using GRIB index files to reduce redundant readings and generate Kerchunk reference files.  

2. Through streaming-like access, convert the reference files into virtual Zarr datasets and utilise Dask compute for scalable data handling   

The methodology utilised recent improvements in the Kerchunk library that integrate GRIB scanning with its index files. This allowed the system to sample subsets of the GRIB corpus instead of processing entire Forecast Model Run Collections (FMRC), significantly optimising performance.  

The workflow was implemented using cloud-based compute operations via Coiled python library and its service on the Google Cloud Platform. Dask cluster, managed through Coiled, enabled the creation of Zarr virtual datasets for analysis and visualisation. This streaming approach efficiently loads weather data into memory on demand, avoiding unnecessary data downloads and duplication.   

We validated the solution with NOAA GFS/GEFS datasets stored in AWS S3 bucket as open datasets. The optimised workflow demonstrated remarkable efficiency, requiring only <5% of the original GRIB data to be read, with the rest replaced by index files as input for reference file creation. This is followed by the step of Kerchunk reference files to virtual Zarr conversion by Dask clusters to process on a regional scale, such as East Africa’s in minutes supporting near real-time applications across spatial and temporal scales.  

This approach significantly enhances post processing workflows for EPS weather forecast, bolstering early warning systems and anticipatory action. Future work will focus on using the method to scaling training datasets and improving the cost efficiency of cGAN training to advance operational early warning systems. This innovative solution directly addresses the challenges faced by meteorological services in processing massive weather datasets, providing a scalable, cost-effective, development foundation for applying GenAI based post-processing and improving early warning systems. 

How to cite: Kalladath, N., Gudoshava, M., Nath, S., Kinyua, J., Cooper, F., Kimani, H., Koros, D., Maswi, C., Mwai, Z., Teshome, A., Abebe, S., Obai, I., Mason, J., Amdihun, A., and Palmer, T.: Weather Data Streaming with Kerchunk: Strengthening Early Warning Systems , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14610, https://doi.org/10.5194/egusphere-egu25-14610, 2025.

EGU25-15406 | Orals | ESSI2.15

Platform Engineering for Earth Observation: A Unified Approach to HPC and Cloud Systems 

Armagan Karatosun and Vasileios Baousis

The growing volume of Earth Observation (EO) and Earth modeling data makes it increasingly impractical to download and analyze it locally. Furthermore, as cloud-native data formats and AI/ML-driven models gain popularity, the community requires powerful computing and storage solutions to efficiently process and analyze EO data. High-performance computing (HPC) and cloud infrastructures can help accomplish this, but both bring significant challenges in maintaining those resources, putting additional workloads on the scientists and developers.

In this paper, we will present our solution, which uses cloud-native technologies and a “Control Plane” approach to seamlessly interact with HPC scheduling endpoints like SLURM and PBS, as well as cloud infrastructure resources, allowing HPC jobs to be submitted and monitored directly from a Kubernetes-based infrastructure. In contrast to traditional IT architecture, Platform Engineering is concerned with lowering operational complexity by introducing control planes to provide self-service capabilities. By abstracting away the complexities of the underlying infrastructure, this method gives teams a customized, scalable, and dependable environment to suit their unique requirements. We will thoroughly analyze existing technologies, including their methodologies, strengths, limits, and potential as universal solutions. Furthermore, we will assess their adaptation to various cloud and HPC infrastructures, providing insights into their suitability for larger applications. 

We will conclude our discussion with practical examples showing how the technical benefits of these two computing paradigms, combined with the Platform Engineering approach, may be effectively used in real-world EO data processing scenarios.

How to cite: Karatosun, A. and Baousis, V.: Platform Engineering for Earth Observation: A Unified Approach to HPC and Cloud Systems, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15406, https://doi.org/10.5194/egusphere-egu25-15406, 2025.

High-resolution regional climate model datasets, such as those produced within the Coordinated Regional Downscaling Experiment (CORDEX) framework, are critical for understanding climate change impacts at local and regional scales. These datasets, with their high spatial and temporal resolution, provide detailed insights into region-specific climate phenomena, including urban heat islands, mountainous climates, and extreme weather events. However, their accessibility and usability are often constrained by technical challenges such as fragmented data storage, inconsistent formats, and limited interoperability.

To address these barriers, we are developing the Climate Service Database (CSD) - a centralized data warehouse designed to streamline the temporal and spatial aggregation of CORDEX datasets for climate service applications. The CSD ingests raw CORDEX datasets and applies automated extraction, transformation, and loading (ETL) workflows to produce analysis-ready datasets tailored to user needs. By leveraging cloud-based infrastructure and adhering to Climate and Forecast (CF) conventions, the CSD ensures consistent, interoperable data products that are optimized for scalable access and analysis.

A core functionality of the CSD is its ability to aggregate datasets at multiple spatial and temporal scales, ranging from daily extremes to decadal averages, and across diverse spatial resolutions (e.g., countries, administrative regions, or watersheds). This capability enables the generation of climate indicators (e.g., hot summer days, heavy precipitation events) that are directly relevant for local decision-making and impact assessments. By providing data in cloud-optimized, analysis-ready formats (ARCO) and offering Software as a Service (SaaS), the CSD significantly lowers the technical barriers for researchers, businesses, and policymakers seeking to access user-tailored climate service datasets.

By centralizing and optimizing the processing of regional climate model datasets, the CSD fosters collaboration across research institutions, public agencies, and climate-tech startups. It enables users to efficiently access consistent and up-to-date data while eliminating the redundancies of localized data storage and processing. This approach also opens new opportunities for applying AI-driven analytics and machine learning models to CORDEX data, paving the way for innovative climate services and applications.

Through its focus on regional climate model datasets, the CSD exemplifies how modern data infrastructures can enhance the usability of high-resolution climate data, empowering stakeholders to develop robust, data-driven adaptation and mitigation strategies in response to the challenges of climate change.

How to cite: Buntemeyer, L.: Advancing Regional Climate Data Accessibility through a Cloud-native Climate Service Database, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16230, https://doi.org/10.5194/egusphere-egu25-16230, 2025.

EGU25-17137 | Orals | ESSI2.15

The Sentinels EOPF Toolkit: Community Notebooks and Plug-ins for using Copernicus Sentinel Data in Zarr format 

Dr. Julia Wagemann, Sabrina Szeto, Emmanuel Mathot, and James Banting

Zarr is a key component of the Pangeo ecosystem and instrumental for effectively accessing and processing multi-dimensional Earth data in cloud-based systems. More and more leading satellite data providers are exploring the transition of their data archives to a cloud environment. 

As part of the ESA Copernicus Earth Observation Processor Framework (EOPF), ESA is in the process of providing access to “live” sample data from the Copernicus Sentinel missions -1, -2 and -3 in the new Zarr data format. This set of reprocessed data allows users to try out accessing and processing data in the new format and experiencing the benefits thereof with their own workflows.

To help Sentinel data users to experience and adopt the new data format, a set of resources called the Sentinels EOPF Toolkit is being developed. Development Seed, SparkGeo and thriveGEO, together with a group of champion users (early-adopters), are creating a set of Jupyter Notebooks, plug-ins and libraries that showcase the use of Sentinel data in Zarr for applications across multiple domains for different user communities, including users of Python, Julia, R and QGIS.

This presentation will give a demo of the first set of notebooks and plugins of the Sentinels EOPF toolkit that were developed and that facilitate the adoption of the Zarr data format for Copernicus Sentinel data users. Additionally, we will give an overview of toolkit developments and community activities that are planned throughout the project period.

How to cite: Wagemann, Dr. J., Szeto, S., Mathot, E., and Banting, J.: The Sentinels EOPF Toolkit: Community Notebooks and Plug-ins for using Copernicus Sentinel Data in Zarr format, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17137, https://doi.org/10.5194/egusphere-egu25-17137, 2025.

EGU25-18285 | ECS | Posters on site | ESSI2.15

Regridding Satellite and Model Data to DGGS (HEALPix) Using the Pangeo Ecosystem 

Justus Magin, Jean-Marc Delouis, Lionel Zawadski, Julien Petiton, Max Jones, and Tina Odaka

Regridding data from diverse sources, such as satellite observations and numerical models, is a critical task in Earth system sciences. Proper interpolation methods are essential to ensure data fidelity when combining or comparing datasets on different grids. This becomes especially relevant in the context of emerging grid systems like Discrete Global Grid Systems (DGGS), specifically HEALPix.

DGGS are spatial reference systems designed to partition the Earth’s surface into a hierarchy of equal-area cells. Unlike traditional latitude-longitude grids, DGGS uses tessellations, such as hexagons, to represent the Earth’s curved surface with minimal distortion. This grid system is particularly suited for handling global-scale geospatial data by providing uniform coverage and resolution, enabling efficient storage, processing, and analysis.

HEALPix (Hierarchical Equal Area isoLatitude Pixelation) is a specific implementation of DGGS widely used in astronomy and Earth sciences. HEALPix divides the sphere into equal-area cells following an iso-latitude structure, making it computationally efficient for operations such as spherical harmonics and multi-resolution analysis. Originally developed for astrophysical applications, it has become increasingly popular in the Earth sciences for representing satellite data, model outputs, and other geospatial datasets in a way that preserves area integrity and facilitates seamless multi-resolution data integration.

By leveraging these grid systems, particularly HEALPix, we can achieve a more accurate and efficient representation of geospatial data.

The Pangeo ecosystem includes an array of powerful regridding tools, each tailored to specific grid types and applications. However, navigating this ecosystem to identify the most suitable tool and workflow can be challenging.

In this presentation, we will show an overview of regridding solutions within Pangeo, highlighting their capabilities and limitations, as well as  their application. We will also demonstrate a practical regridding workflow using model outputs or simulated satellite data such as the Odysea dataset (Aviso+ Altimetry. (n.d.). Simulated Level-2 Odysea Dataset. Retrieved from https://www.aviso.altimetry.fr/en/data/products/value-added-products/simulated-level-2-odysea-dataset.html on January 14, 2025), to the HEALPix grid. This workflow will make use of recent advances in technology to make it reproducible to make it efficient and reproducible, such as virtualizarr for fast metadata access and dask for scalable operations, with the output saved as chunked zarr files for seamless integration with downstream analysis.

How to cite: Magin, J., Delouis, J.-M., Zawadski, L., Petiton, J., Jones, M., and Odaka, T.: Regridding Satellite and Model Data to DGGS (HEALPix) Using the Pangeo Ecosystem, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18285, https://doi.org/10.5194/egusphere-egu25-18285, 2025.

EGU25-18336 | Posters on site | ESSI2.15

Advancing Earth System Science through collaboration: An overview of ECMWF Special Projects 

Milana Vuckovic and Becky Hemingway

ECMWF has been providing resources on its operational high-performance computing (HPC) and cloud facilities (European Weather Cloud) to researchers and institutions through the Special Projects framework. This framework has been established almost 50 years ago as part of the creation of ECMWF. ECMWF's HPC facility is specifically designed to support both operational time-critical production of global weather forecasts and typical research workflows, therefore through Special Projects, researchers can get access not only to a top high-performance computing and cloud facility and one of the largest meteorological archives in the world, but also full user support.
Special Projects are defined as experiments or investigations of a scientific or technical nature, undertaken by one or more ECMWF Member States, likely to be of interest to general scientific community. The main aim of this initiative is to facilitate collaboration, enabling the development of innovative methodologies and tools for numerical weather prediction, climate and environmental modelling, and other disciplines within Earth System Sciences. All Special Project applications undergo a review process by ECMWF and its Scientific Advisory Committee (SAC), as well as ECMWF Member State's meteorological services and are ranked primarily by their scientific quality.
This poster will describe the Special Projects framework and showcase three recent Special Projects that illustrate collaborative nature of the initiative using ECMWF's HPC and European Weather Cloud facilities, including validating ICON model on ECMWF systems, the development of next-generation European Earth System Model (EC-EARTH4) and mapping the yet uncharted continuum of cyclone dynamics for the Euro Atlantic domain.
Through these examples, the poster will demonstrate how ECMWF Special Projects foster international collaboration, resource sharing, and innovation, enabling advancement in Earth System Science. 

How to cite: Vuckovic, M. and Hemingway, B.: Advancing Earth System Science through collaboration: An overview of ECMWF Special Projects, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18336, https://doi.org/10.5194/egusphere-egu25-18336, 2025.

EGU25-20590 | Posters on site | ESSI2.15

Dhemeter: Data Hub for Environmental and METEorological Resources 

Cédric Pénard, Nathan Amsellem, Boris Gratadoux, Bastien Barthet, Jean Christophe Pere, Johannes Staufer, Laure Chaumat, and Alexia Mondot

Dhemeter is a weather and environmental data aggregator. It is developed using a microservices architecture to handle a wide variety of data from various providers, such as NOAA, ECMWF, Eumetsat, Météo-France, DWD, and Copernicus. The implementation of aggregation, concatenation, and consistency functionalities has been successfully executed for meteorological data. This versatile tool accommodates numerical model data, in-situ observations, remote sensing data, and reanalyses, allowing for online data retrieval from multiple sources.

Key features of the aggregator include:

  • Concatenation of Multiple Data Sources: Users can combine data according to selected categories such as Observations, Forecasts, and Reanalyses.
  • Standardization of Physical Data: This involves spatial and temporal interpolation as well as geographical selections to ensure uniformity.
  • Storage of Resulting Data Structures: The data is stored in a pivot format that facilitates access and distribution of scientific data, specifically in the NetCDF format.

The microservices architecture of the aggregator allows for the extensibility of the offered data catalog, and an API is available for users to make direct queries to chosen data sources.

In the short to medium term, the goal is to enhance the tool further, evolving it into a comprehensive data distribution and aggregation system that centralizes and simplifies access to various types of data, including meteorological, oceanographic, and air quality data.

Dhemeter focuses on ease of use, extensibility, scalability, and customization, offering users capabilities for data fusion and harmonization.

How to cite: Pénard, C., Amsellem, N., Gratadoux, B., Barthet, B., Pere, J. C., Staufer, J., Chaumat, L., and Mondot, A.: Dhemeter: Data Hub for Environmental and METEorological Resources, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20590, https://doi.org/10.5194/egusphere-egu25-20590, 2025.

EGU25-20676 | Orals | ESSI2.15

Integrated geospatial Python libraries for efficient analysis of modern elevation measurements 

Scott Henderson, David Shean, Jack Hayes, and Shashank Bhushan

NASA established the Surface Topography and Vegetation (STV) Incubation program to develop and mature the next-generation measurement approaches to precisely map Earth’s changing surface and overlying vegetation structure, and prepare for a dedicated satellite mission within the next decade. Over the past two decades, large archives of 3D surface elevation measurements by airborne and satellite instruments including LiDAR, altimeters, Synthetic Aperture Radar, and stereo optical imagery have been systematically collected, though not always in a coordinated way. Yet, many of these datasets are fortuitously acquired over the same location within a short temporal window (e.g., <1-14 days) and many are now publicly available and hosted on the cloud. In theory, this is a great opportunity to synthesize myriad elevation measurements for STV researchers, but in practice merging these datasets accurately for scientific analysis requires dealing with numerous data formats, complex 4D coordinate reference systems, and securing access to significant computational resources.

We are developing an open-source Python library to identify, curate, and efficiently process coincident elevation measurements spanning the last several decades. This work would not be possible without well-integrated geospatial libraries (e.g. Geopandas, Xarray, Dask), as well as emerging cloud-native data and metadata formats such as Cloud-Optimized Geotiff and STAC-GeoParquet. We will describe our work to-date and reflect on the process of collaborative development across libraries, on our increasing reliance on Cloud resources, and current and future research directions.

How to cite: Henderson, S., Shean, D., Hayes, J., and Bhushan, S.: Integrated geospatial Python libraries for efficient analysis of modern elevation measurements, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20676, https://doi.org/10.5194/egusphere-egu25-20676, 2025.

EGU25-21202 | Orals | ESSI2.15

From SAFE to Zarr: The EOPF Sample Service Initiative 

Christian Briese, Christoph Reimer, Christian Briese, Christoph Reck, Dimitrios Papadakis, Michele Claus, Gunnar Brandt, Anne Fouilloux, and Tina Odaka

Over the past decade, the operational Copernicus Sentinels Data Processors have generated vast amounts of Earth observation data, supporting various scientific and commercial applications. However, the current format used by ESA to provide Copernicus data, known as SAFE (Standard Archive Format for Europe), has become outdated. To address this, ESA has initiated the transition to a new Zarr-based data format. The Earth Observation Processing Framework (EOPF) Sample Service is ESA’s official initiative to support this transition by providing early access to the new format for users. This shift is essential for creating a cloud-native and interoperable solution that enhances data accessibility and integration with modern processing frameworks. The primary goal is to standardize data formats across Sentinel missions, enable scalable processing on cloud platforms, and ensure compatibility with contemporary data science tools. This initiative is crucial for minimizing disruption and ensuring continuity for users, applications, and services built around existing data formats.

The EOPF Sample Service comprises several key components. The EOPF Core Platform re-formats ingested SAFE data products into the new cloud-optimized EOPF Zarr data products and provides data access via STAC API and S3 API. To ensure timely conversion, the platform utilizes Argo Events and the Copernicus Data Space Ecosystem's subscription service. This platform is maintained by experts from EODC and DLR. The EOPF User Platform offers additional user services, including JupyterHub (BinderHub), Dask, and a STAC Browser, which are essential for supporting user adoption by lowering the entrance barrier to cloud applications and data discovery capabilities. The service is designed to make use of advanced technologies such as Kubernetes for container orchestration and Dask for parallel computing. User and identity management is achieved in cooperation with the Copernicus Data Space Ecosystem.

User adoption is further facilitated through Jupyter Notebooks designed by experts within the consortium, including members from the Pangeo community. These notebooks showcase the use of the new format within the community and are continuously improved by incorporating user feedback. In addition, enhancements are made to widely-used software tools like GDAL to support the new format, with practical demonstrations available through Jupyter Notebooks. The consortium selected by ESA to carry out this implementation includes experts from Brockmann Consult, DLR, Ifremer, EURAC, Evenflow, Simula, and EODC, each contributing their specialized knowledge in Earth observation, data management, and user engagement.

This contribution aims to present the EOPF Sample Service initiative and the current status of its implementation. The first Jupyter Notebooks demonstrating the new format will also be showcased, providing users with an intuitive and user-friendly interface for accessing and processing sample data in the new EOPF format.

How to cite: Briese, C., Reimer, C., Briese, C., Reck, C., Papadakis, D., Claus, M., Brandt, G., Fouilloux, A., and Odaka, T.: From SAFE to Zarr: The EOPF Sample Service Initiative, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21202, https://doi.org/10.5194/egusphere-egu25-21202, 2025.

EGU25-21279 | Orals | ESSI2.15

Advancing Cloud-Native Data Analysis and Publishing with Pangeo Tools in EarthCODE 

Deyan Samardzhiev, Anne Fouilloux, Tina Odaka, and Benjamin Ragan-Kelley

EarthCODE (Earth Science Collaborative Open Development Environment) is a platform that leverages cloud-native tools to empower Earth system researchers in accessing, analyzing, and sharing data across distributed infrastructures, such as the Copernicus Data Space Ecosystem and Deep Earth System Data Laboratory (DeepESDL). By integrating Pangeo ecosystem tools—including Xarray, Dask, and Jupyter—EarthCODE supports scalable, FAIR-aligned workflows tailored to the challenges of Earth system science.

EarthCODE streamlines cloud-based data analysis and publishing by enabling collaborative research through interoperable workflows for analyzing complex datasets, including satellite observations, climate models, and in-situ measurements. Researchers can publish their analyses and workflows as reusable, executable resources in EarthCODE’s science catalog, fostering alignment with open science principles.

Through its integration of Pangeo tools, EarthCODE offers an intuitive environment for reproducibility, scalability, and collaboration, bridging the gap between data analysis and actionable insights. This presentation will demonstrate EarthCODE’s capabilities, including live, executable Jupyter notebooks that highlight its potential for sharing workflows and engaging diverse user groups. EarthCODE exemplifies the transformative power of cloud-native research, promoting open science and advancing the accessibility of Earth system data.

How to cite: Samardzhiev, D., Fouilloux, A., Odaka, T., and Ragan-Kelley, B.: Advancing Cloud-Native Data Analysis and Publishing with Pangeo Tools in EarthCODE, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21279, https://doi.org/10.5194/egusphere-egu25-21279, 2025.

EGU25-21603 | ECS | Orals | ESSI2.15 | Highlight

The Pangeo Ecosystem Supporting Climate Change Adaptation: The FAIR2Adapt RiOMar Case Study 

Even Moa Myklebust, Ola Formo Kihle, and Justus Magin

The RiOMar (River dominated Ocean Margins) case study, part of the FAIR2Adapt (FAIR to Adapt to Climate Change) project (EU funded project grant agreement No 101188256), focuses on supporting science-based climate change adaptation strategies for coastal water quality and marine ecosystem management. The case study uses large environmental datasets, such as sea temperature, salinity, and other marine parameters, to assess and model the impacts of climate change on coastal ecosystems. As part of the FAIR2Adapt project, which aims to enhance the shareability, accessibility, interoperability, and reusability of environmental data through the FAIR (Findable, Accessible, Interoperable, and Reusable) principles, the RiOMar case study emphasizes the use of cutting-edge data processing and analysis methods to support adaptive strategies for climate resilience.

In this presentation, we present our approach to reading the RiOMar large environmental datasets in netCDF format, creating VirtualZarr archives for efficient data handling, transforming them into a Discrete Global Grid System (DGGS) using the Healpix grid.Leveraging the Pangeo ecosystem, we use tools such as Kerchunk to create simpler access to multiple data sources, parallelize dataset processing using Dask or Cube, enabling scalable analysis of these complex, multi-dimensional data. We will show a comparison of performance between traditional cube-based approaches and Dask, highlighting the advantages of parallelized processing. Furthermore, we will showcase how to interactively visualize these datasets using tools like XDGGs and Lonboard, facilitating seamless exploration and analysis of the underlying environmental patterns. This work underscores the potential of open-source tools, scalable computing techniques, and the Pangeo ecosystem to enhance the accessibility and usability of large geospatial datasets in climate adaptation research.

How to cite: Moa Myklebust, E., Formo Kihle, O., and Magin, J.: The Pangeo Ecosystem Supporting Climate Change Adaptation: The FAIR2Adapt RiOMar Case Study, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21603, https://doi.org/10.5194/egusphere-egu25-21603, 2025.

Statistical models are a frequently used tool in hydrology, especially when it comes to estimating design floods, i.e. flood events that used to design flood protection systems or reservoirs. The often complex hydrological data, which are affected by e.g. missing values, extremes or time-varying processes, require sophisticated statistical models that take these challenges into account. As a scientist, developing such models can be a lot of fun and provide interesting insights. After months of thinking about the best model under certain statistical assumptions, proving asymptotic theorems and testing the model with synthetic data, you are happy and proud to have developed a new model. This model will hopefully be widely used in future research. The next step is to apply the model to a large real data set. The results look good on average. The results will be shared with practitioners, because of course you want the model to be useful for science and practice. And then: the phone call. You are told that your results are not plausible for a certain catchment area. And in general, the new model is not needed in practice because there is an established model. This example describes such a case and discusses ways of dealing with it. It is intended to illustrate the importance of communication between science and practice and a general understanding between both sides.

How to cite: Fischer, S.: When practical considerations impact your scientific model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1620, https://doi.org/10.5194/egusphere-egu25-1620, 2025.

EGU25-1660 | Orals | EOS4.8

The Minkowski–Bouligand dimension of a clay brick 

Nick van de Giesen and John Selker

In the early 1990's, fractals and chaos were hot. In 1987, James Gleick had published "Chaos: Making a New Science", popularizing non-linear dynamics. Hydrologists played an important role in the development of fractal theory. Hurst had discovered that sequences of dry and wet years for the Nile showed very long memory effects. Instead of the chance of a dry year following a dry year being 50%, Hurst found that there were surprisingly many long series of dry or wet years. Seven fat years, seven lean years, as it is noted in Genesis. Scott Tyler found fractals in soils ("Fractal processes in soil water retention"). At Cornell, where we were at the time, David Turcotte described "Fractals in geology and geophysics". A few years later, Ignacio Rodríguez-Iturbe and Andrea Rinaldo would publish "Fractal River Basins: Chance and Self-Organization". In short, fractals were exciting scientific gold.

A fractal is not just an obscure mathematical object but something that can actually be found everywhere in nature. Early on, a paper was published in Nature with the title "Fractal viscous fingering in clay slurries" by Van Damme, Obrecht, Levitz, Gatineau, and Laroche. They "only" did an experiment on a fractal embedded in 2D; we should be able to do one better and find the fractal dimension of the surface of cracking clay embedded in 3D. So out we went, collected some clay, mixed it with water in a cement mixer, siliconed together a shallow "aquarium", and poured in the slurry. To observe the cracking of the drying slurry, a video camera was mounted above the experiment, looking down and taking time-lapse images. To access the views from the sides, mirrors were installed at 45 degrees at each of the four sides. Lights made sure the camera captured high quality images. The whole set-up was enclosed in a frame with dark cloth to ensure that lighting was always the same.  We already had some box-counting code ready to calculate the fractal dimension of the surface, called the Minkowski–Bouligand dimension. One variable needed some extra attention, namely the boundary between the clay slurry and the glass sides. If the clay would cling to the sides, it would be difficult to understand the effects that this boundary condition had on the outcome of the experiment. Moreover, the cracks may not have become visible in the mirrors when the sides were covered with mud. So, instead, it was decided to make the sides hydrophobic with some mineral oil. This ensured that when the clay would start to shrink, it would come loose from the sides. Now, all we had to do was wait. It took only a week or so before the consolidated slurry started to shrink and to come loose from the sides. After that, the clay continued shrink for many weeks. This is how we learned that the fractal dimension of a shrinking brick of clay is (very close) to 3.0. 

How to cite: van de Giesen, N. and Selker, J.: The Minkowski–Bouligand dimension of a clay brick, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1660, https://doi.org/10.5194/egusphere-egu25-1660, 2025.

EGU25-5035 | Orals | EOS4.8

Landslides and hillslope erosion increase relief 

Stefan Hergarten and Jörg Robl

In 2018, we found exciting new results in landform evolution modeling by coupling the two simplest models of fluvial erosion and hillslope processes. While the stream-power incision model is the simplest model for detachment-limited fluvial erosion, the diffusion equation is the simplest description of hillslope processes at long timescales. Both processes were added at each grid cell without an explicit separation between channels and hillslopes because fluvial erosion automatically becomes dominant at large catchment sizes and negligible at small catchment sizes.

We found that increasing diffusion reduces the relief at small scales (individual hillslopes), but even increases the large-scale relief (entire catchments). As an immediate effect, the hillslopes become less steep. In turn, however, we observed that the network of the clearly incised valleys, which indicates dominance of fluvial erosion over diffusion, became smaller. So a smaller set of fluvially dominated grid cells had to erode the material entering from the hillslopes. To maintain a morphological equilibrium with a given uplift rate, the rivers had to steepen over long time. This steepening even overcompensated the immediate decrease in relief of the hillslopes.

This result was counterintuitive at first, but we were happy to find a reasonable explanation. So we even prepared a short manuscript for a prestigious  journal. We just did not submit it because we wanted to explain the effect quantitatively from the physical parameters of the model. From these theoretical considerations, we found that our numerical results did not only depend on the model parameters, but also on the spatial resolution of the model and noticed that this scaling problem was already discussed in a few published studies. Beyond the scaling problem, we also realized that applying the concept of detachment-limited fluvial erosion to the sediment brought from the hillslopes into the rivers is quite unrealistic. A later study including fluvial sediment transport and a model for hillslope processes that avoids scaling problems did not predict any increase in large-scale relief. So we finally realized that our original findings were mainly the result of a specific combination of models that should not be coupled this way and are not  as relevant for landform evolution as we thought.

This example illustrates many of the pitfalls of numerical modeling beyond purely technical issues. In particular, combining models that are widely used and make sense individually may still cause unexpected problems.

 

How to cite: Hergarten, S. and Robl, J.: Landslides and hillslope erosion increase relief, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5035, https://doi.org/10.5194/egusphere-egu25-5035, 2025.

EGU25-5091 | ECS | Orals | EOS4.8

(Re)(De)bugging tragedies with Hector 

Guillemette Legrand

In this presentation, I will discuss my research into the simple climate model Hector, which calculates temperature change based on the impact of various climate scenarios. More specifically, I will discuss how an artistic-led approach through (un)voluntary-caused computational bugs can help document the model's logic and socio-political implications. I will describe methods for collective 'debugging' to produce transdisciplinary knowledge (beyond solely scientific inquiry) to foster conversation about the potential and limits of current climate infrastructure to foster concrete climate actions. This research investigates the field of climate science through artistic practice, software and infrastructure studies, and participatory methods. To expand on the role of bugs in my investigation, I will elaborate on concrete examples of differences in perception of 'error' in the fields of arts and science, looking at case studies where mistakes or glitches have been valorised and mobilised through artistic practice to grapple with, appropriate, and/or repurpose scientific instruments.

How to cite: Legrand, G.: (Re)(De)bugging tragedies with Hector, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5091, https://doi.org/10.5194/egusphere-egu25-5091, 2025.

EGU25-5951 * | Orals | EOS4.8 | Highlight

Improving extreme temperature definitions until they are wrong 

Lukas Brunner, Maximilian Meindl, and Aiko Voigt

"Doesn't this look a bit strange?" 

It began with an innocent question during one of our Master's colloquia. And it could have ended there. "We were just following an approach from the literature". And who could argue against following the literature?

But it bugged me. During a long train ride, I began to think about the issue again. 10 hours and many papers later, I was only more confused: was it really that obvious, and why had no one picked up on it before? But sometimes the most obvious things are the most wicked, and after a few conversations with knowledgeable colleagues, I was sure we were in for an unexpected surprise. 

A commonly used approach to defining heat extremes is as exceedances of percentile-based thresholds that follow the seasonal cycle. Such relative extremes are then expected to be evenly distributed throughout the year. For example, over the 30-year period 1961-1990, we expect three (or 10%) of January 1s to exceed a 90th percentile threshold defined for the same period - and the same for all other days of the year. In a recent study, we show that there are many cases where this does not hold, not even close (Brunner and Voigt 2024).

Here, we tell the story of how this blunder spread in the literature out of the desire to improve extreme thresholds. We show that seemingly innocent changes can sometimes have unintended consequences and that taking the time to check the obvious can help avoid mistakes in science. 

 

Brunner L. and Voigt A. (2024): Pitfalls in diagnosing temperature extremes, Nature Communications, https://doi.org/10.1038/s41467-024-46349-x

How to cite: Brunner, L., Meindl, M., and Voigt, A.: Improving extreme temperature definitions until they are wrong, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5951, https://doi.org/10.5194/egusphere-egu25-5951, 2025.

When economists estimate the expected economic damages from current-day CO2 emissions, they usually calculate the social cost of carbon – that is, the aggregated damage caused by the emission of an additional ton of CO2. Several cost-benefit integrated assessment models (IAMs) are built to assess this quantity, and among them is the META model. This model is built specifically to assess the effects of tipping points on the social cost of carbon, and it usually operates stochastically. When integrating a deterministic, but small carbon cycle tipping point into the model, however, the social cost of carbon seems to explode: a few gigatons of additional emissions almost double the impact estimates of CO2 emissions! Well, maybe. In fact, these results are a pure artifact of two things: 1) the way in which social cost of carbon estimates are calculated with IAMs; and 2) the way that tipping points are implemented in the META model. And, of course, 3): a lack of initial thoughtfulness on behalf of myself. A thorough look into this issue shows that, as expected, a marginal change in emissions leads to a marginal change in damage estimates. While that result is rather boring, the previous blunder can actually be instructive about the scarcely-known methods used to obtain economic impact estimates of climate change.

How to cite: Schaumann, F.: Drastic increase in economic damages caused by a marginal increase in CO2 emissions?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9145, https://doi.org/10.5194/egusphere-egu25-9145, 2025.

EGU25-10285 | ECS | Orals | EOS4.8

How robust are modeled non-local temperature effects of historical land use changes really? 

Felix Jäger, Petra Sieber, Isla Simpson, David Lawrence, Peter Lawrence, and Sonia I. Seneviratne

Historically, large areas across the globe have been affected by deforestation or irrigation expansion. The replacement of forests with agricultural land and increased water availability in irrigated croplands altered the land’s surface properties, leading to influences of biogeophysical changes on near-surface temperature. From limited observations and mostly idealized simulations, we know that sufficiently large alterations of land surface properties can theoretically lead to systematic temperature and precipitation changes outside and even far from the altered areas. Not only the advection of temperature anomalies, but also changes in circulation and ocean feedbacks have been shown to be potential drivers of such non-local responses in single and multi-model studies.

We tested the robustness of non-local temperature signals to internal variability in the fully coupled Community Earth System Model 2 (CESM2) simulations of the historical period (1850 – 2014) with all forcings vs. all-but-land-use-change forcings. Doing so, we first found seemingly robust non-local temperature effects of land use change on the global and regional scale. But when accounting for the sampling of internal variability in the model using a large initial condition ensemble, the global scale signal was found to be indistinguishable from noise. Only regionally in some hotspots, we found robust and historically important non-local temperature signals. Through increasingly rigorous analysis, we reached a partly negative and unexpected but important finding, which may have implications for future assessments of comparably weak or spatially heterogeneous forcings to the Earth system.

How to cite: Jäger, F., Sieber, P., Simpson, I., Lawrence, D., Lawrence, P., and Seneviratne, S. I.: How robust are modeled non-local temperature effects of historical land use changes really?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10285, https://doi.org/10.5194/egusphere-egu25-10285, 2025.

EGU25-10615 | Orals | EOS4.8

Think twice – pitfalls in hydrological modelling 

Jan Seibert, Franziska Clerc-Schwarzenbach, Ilja van Meerveld, and Marc Vis

Failures are only common in science, and hydrological modelling is no exception. However, we modellers usually do not like to talk about our mistakes or our overly optimistic expectations and, thus, “negative” results usually do not get published. While there are examples where model failures indicated issues with the observational data, in this presentation the focus is on modelling studies, where some more (realistic) thinking could have helped to avoid disappointments. Examples include the unnecessary comparison of numerically identical model variants, naively optimistic expectations about increasing the physical basis of bucket-type models and excessively hopeful assumptions about the value of data.

How to cite: Seibert, J., Clerc-Schwarzenbach, F., van Meerveld, I., and Vis, M.: Think twice – pitfalls in hydrological modelling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10615, https://doi.org/10.5194/egusphere-egu25-10615, 2025.

EGU25-11357 | Orals | EOS4.8

Two steps forward, one step back: four years of progress and setbacks on invisible ship tracks 

Peter Manshausen, Anna Tippett, Edward Gryspeerdt, and Philip Stier

The idea of invisible ship tracks for the study of aerosol-cloud interactions sounds promising: We have been studying the effects of aerosols on clouds for many years, among others by investigating the bright lines of clouds left in low marine clouds by ships. However, only a small fraction of ships leaves behind visible tracks. This means we can only study aerosol-cloud interactions under certain meteorological conditions, biasing our understanding. Instead, by studying all clouds polluted by ships ('invisible ship tracks') with a methodology we developed, we should be able to get a full picture of aerosol-cloud interactions. A number of interesting and impactful results have come out of this research, along with several setbacks and corrections to initial results. Here, we examine them in order, showing how correcting for one identified bias can introduce two new ones. Unexpected glitches arise from sources as varied as: choices regarding ship track definition, retrieval geometry, specific weather systems biasing results, and mathematical subtleties. What can we conclude after four years of progress on this methodology? While some results still stand, others had to be significantly corrected. This makes us see invisible ship tracks as an example of research that is closer to a method of 'tinkering' than to a 'magnificent discovery'.

How to cite: Manshausen, P., Tippett, A., Gryspeerdt, E., and Stier, P.: Two steps forward, one step back: four years of progress and setbacks on invisible ship tracks, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11357, https://doi.org/10.5194/egusphere-egu25-11357, 2025.

EGU25-12720 | ECS | Posters on site | EOS4.8

Physical understanding of bugs to improve the representation of the climate system   

Hans Segura, Cathy Hohenegger, Reiner Schnur, and Bjorn Stevens

Earth system models are important tools used to understand our climate system and project possible changes in our climate due to anthropogenic and natural forcings. Human errors can occur in the development of Earth System models, i.e., bugs, giving an unphysical representation of our climate. A way to identify and solve bugs is to apply physical concepts. Here, we present an experience that occurred in the development of the ICOsahedral Non-hydrostatic model (ICON) as a kilometer-scale Earth System model, in which physically understanding a bug in the surface energy budget fixed land precipitation. 

In a simulation of ICON, referred to as ICON-bug, precipitation over tropical land continuously decreased across the simulation. This led to a ratio of land-ocean precipitation in the tropics of less than 0.7, which, otherwise, should be more than 0.86. As part of the possible explanations, the surface energy budget over land was targeted as a culprit. This idea relies on the influence of the interaction between soil moisture, surface heat fluxes, and winds to generate circulation favoring precipitation over dry land surfaces (Hohenegger and Stevens 2018). Indeed, the surface energy budget over dry surfaces in the ICON-bug showed an error in sensible heat flux. The sensible heat flux transmitted to the atmosphere was 70% of what was calculated for the surface module. Fixing this error closed the surface energy budget and increased land precipitation over the tropics, leading to a ratio of land-ocean precipitation of 0.94, close to observations. 

How to cite: Segura, H., Hohenegger, C., Schnur, R., and Stevens, B.: Physical understanding of bugs to improve the representation of the climate system  , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12720, https://doi.org/10.5194/egusphere-egu25-12720, 2025.

Whenever you study a phenomenon of mm to a few cm-scale in the laboratory which involves an interface, the question of surface tension arises. Surface tension is due to the fact that molecules prefer to stay with their own kind. Therefore, the creation of an interface between two fluids requires energy, and this influences the dynamics around the interface.

Surface tension can be a blessing: it produces the round shape of rain drops or the nice bubble shapes of colorful liquid in a lava lamp. It allows objects with a higher density to float on a liquid (such as an insect on water, or a silicone plate on sugar syrup). It can generate flow up a capillary.

However, it can also be a curse in the case of thermal convection. Purely thermal convection  develops when a plane layer of fluid is heated from below and cooled from above. The engine of motion is the thermal buoyancy of the fluid. This is what is happening in a planetary mantle on scales of hundreds to thousands kilometers. This is also what is happening in a closed box in the laboratory. But as soon as an interface exists, either between an upper and a lower experimental mantle, or in the case of a free surface at the top of the fluid layer, surface tension effects can become important. For exemple, the variation of surface tension with temperature was responsible for the beautiful honey-comb patterns imaged by Benard (1901) in the first systematic study of thermal convection with a free-surface. Surface tension is also going to act against the initiation of subduction (which acts to break the surface). 

We shall review in this presentation the signatures of surface tension in a convective context, and the different ways to minimize and/or remove the effects of surface tension in convection experiments, such as using miscible liquids, or a layer of experimental « sticky air ».

How to cite: Davaille, A.: Analog studies of mantle convection: the curse of surface tension (or not) ?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15059, https://doi.org/10.5194/egusphere-egu25-15059, 2025.

EGU25-15457 | Orals | EOS4.8

The crux with variability: too much or too little 

Markus Weiler

In hydrology we measure and follow the water. What if there is too much or too little? It happens a lot. As a field hydrologist, I frequently have to determine the location of a measurement, the time to take the measurement, the location to set up a field experiment, or the amount of a tracer to inject to study a hydrological system. However, this is a very bumpy road, as variability is often not in favor of my decisions because the distribution is wider than expected, bimodal instead of unimodal, or the probability of an event is theoretically small, but still an extreme event occurs during our experiment. I will showcase some examples to demonstrate what I mean and what I experienced, as well as how frequently the PhD students or Postdocs have suffered as a result of my decisions or of the unexpected variability: Climatic variability resulted in a winter without snow, just as new sensors were already deployed. Or the winter snowpack was extremely high, preventing any work at high altitudes in the Alps until mid of July, thereby reducing our field season by half. An ecohydological study to observe the effects of drought in a forest with a rainout shelter was ineffective because it occurred during an extremely dry year, making the control just as dry as our drought treatment. The automatic water sampler was set-up to collect stream water samples, but it was washed away four weeks later by the 50-year flood. The calculated amount of artificial tracer was either way too low, because the transit times of the system were much longer than expected, or it was far too high, resulting in colored streams or samples that had to be diluted by a factor of 100 due to much faster transit times Finally, and most expensively, we installed many trenches along forest roads to measure subsurface stormflow but after three years, we abandoned the measurements because we never measured a drop of water coming out of the trenches, as the bedrock permeability was much higher due to many high permeable fissures that prevented the formation of subsurface stormflow.  These experiments or observations failed because of unexpected variability in input, system properties or a lack of technical variability in the equipment. I will reflect on residual risk of failure in fieldwork related to that crux and discus approaches to reduce this risk.

How to cite: Weiler, M.: The crux with variability: too much or too little, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15457, https://doi.org/10.5194/egusphere-egu25-15457, 2025.

EGU25-15826 | ECS | Posters on site | EOS4.8

Output regridding can lead to Moiré pattern in km-scale global climate model data from ICON 

Benjamin Poschlod, Lukas Brunner, Benjamin Blanz, and Lukas Kluft

The emergence of global km-scale climate models allows us to study Earth's climate and its changes with unprecedented local detail. However, this step change in spatial resolution to grid spacings of 10 km or less also brings new challenges to the numerical methods used in the models, the storage of model output, and the processing of the output data into actionable climate information. The latest versions of the ICON-Sapphire model developed in the frame of the NextGEMS project address these challenges by running on an icosahedral grid while outputting data on the so-called HEALPix grid. Both grids are unstructured grids, which avoids, for example, the issue of longitude convergence. In addition, HEALPix allows data to be stored in a hierarchy of resolutions at different discrete zoom levels, making it easier for users to handle the data.  

The transition from the native 10 km grid to the output grid is made by a simple but very fast nearest-neighbour remapping. An advantage of this simple remapping approach is that the output fields are not distorted, i.e. the atmospheric states in the output remain self-consistent. As HEALPix only provides discrete zoom levels in the setup of the run, it was decided to remap to the closest available resolution of 12 km rather than to the next finer resolution of 6 km. This decision was made to avoid artificially increasing the number of grid points and to avoid creating duplicates through the nearest neighbour remapping.

As a consequence of this approach, wave-like patterns can emerge due to the Moiré effect that can result from the interaction of two grids. We find these patterns when looking at certain derived precipitation extremes, such as the annual maximum daily precipitation, the 10-year return level of hourly precipitation, or the frequency of dry days. At first, we interpreted these patterns as a plotting issue, as the figures might have too low resolution to cope with the high-resolution global plot (aliasing) leading to a Moiré pattern.

However, zooming in on the affected regions and closer examination of the data revealed that the pattern is in fact in the data. Further investigation with synthetic data confirmed the suspicion that the Moiré pattern was indeed caused by the remapping of the native 10 km icosahedral grid to the slightly coarser 12 km HEALPix grid. We hypothesise that precipitation is particularly affected by this issue, as it typically contains many grid cells with zero precipitation, with local clusters of non-zero values at the 15-minutely output interval. Yet, we cannot exclude the possibility that other variables are also affected.

As a consequence, if remapping is required, it is recommended to first remap from the native resolution to a finer resolution grid. As a next step, the conservative nature of the HEALPix hierarchy can be used to compute the coarser level. In this way it is likely to be possible to avoid aliasing and still keep the amount of output data the same.

How to cite: Poschlod, B., Brunner, L., Blanz, B., and Kluft, L.: Output regridding can lead to Moiré pattern in km-scale global climate model data from ICON, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15826, https://doi.org/10.5194/egusphere-egu25-15826, 2025.

EGU25-17676 | ECS | Posters on site | EOS4.8

What river plastic hotspots do not have in common 

Rahel Hauk, Adriaan J. Teuling, Tim H.M. van Emmerik, and Martine van der Ploeg

Plastic pollution is a global issue, across all environmental compartments. Rivers connect the terrestrial with the marine environment, and they transport various materials, among these plastic pollution. Rivers not only transport plastic, but also accumulate and store it, especially on riverbanks. In fact, plastic deposition and accumulation on riverbanks is a common occurrence. However, our understanding of why plastic is deposited on a certain riverbank is rather limited. Riverbanks along all major Dutch rivers have been monitored for plastic and other litter twice a year by citizen scientists, in some locations since 2018. This provides an extensive dataset on plastic accumulation, and we used these data with the aim of understanding the factors determining plastic concentration/accumulation variability over time and space. We tested multiple riverbank characteristics, such as vegetation, riverbank slope, population density, etc., hypothesized to be related to plastic litter. After having exhausted a long list of auxiliary data and analysis strategies, we found no significant results. Ultimately, we had a close look at ten consistent hotspots of macroplastic litter, along the Meuse, and Waal river. And once again, they seem to have nothing in common. But, there is a pattern, because some riverbanks have consistently very high densities of plastic litter so it does not seem completely random. We have been looking to explain spatial variability, whereas we might have to look at temporal consistency, and we shall not give up our efforts to bring order to this chaos.

How to cite: Hauk, R., Teuling, A. J., van Emmerik, T. H. M., and van der Ploeg, M.: What river plastic hotspots do not have in common, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17676, https://doi.org/10.5194/egusphere-egu25-17676, 2025.

EGU25-17811 | Posters on site | EOS4.8

Temporal variation of ambient noise at the Grande Dixence reservoir recorded by a nodal deployment 

Mita Uthaman, Laura Ermert, Angel Ling, Jonas Junker, Cinzia Ghisleni, and Anne Obermann

Grande Dixence, the tallest gravity dam in the world, is located in the Swiss Alps on the Dixence River with a catchment area of 4 km2 at a towering elevation of 2000m. The lake serves as a collecting point of melt water from 35 glaciers and reaches full capacity by late September, subsequently draining during winter and dropping to lowest levels in April. For a reservoir as large as the Grande Dixence, the variation in hydrological load can be expected to induce changes in crustal stress. The goal of this study was to harness the loading effect of the time-varying level of reservoir load as a source of known stress to investigate the variation in seismic velocity of the bedrock due to changes induced in crustal stress and strain rates. 22 seismic nodes were thus deployed along the banks of the reservoir which were operational from mid-August to mid-September, corresponding to the time period when the lake level reaches its maximum. Of the 22 nodes, 18 were deployed in closely spaced patches of six in order to carry out coherent stacking and to increase the signal-to-noise ratio, besides one group of three nodes and one single node. Measurement quality appears satisfactory: small local earthquakes are recorded well, and the probabilistic power spectral densities (PPSDs) computed for data quality validation evidence the ambient noise levels to be well within the global noise limits. However, the recorded noise is unexpectedly complex and, at periods shorter than 1 second, varies strongly by location. The 0.5--5s (0.2--2 Hz) period band at lakes generally records a diurnally varying noise level, often associated with lake generated microseism. Diurnal variations around 1 second of period are observed in our study as well. The amplitude of ambient noise level around 1 second of period is observed to be highest when the lake level changes, along with the prominent diurnal variation. A similar variation is observed in the seismic velocity variation (dv/v) computed from cross-correlated and auto-correlated ambient noise filtered between 0.5--1 Hz, with dv/v exhibiting a drop with rising lake level. These results provide preliminary evidence for possible change in crustal stress state with changing hydrological load. Future direction of this study consists of analytically modeling the results to quantify the influence of thermobarometric parameters on PPSDs and dv/v, and deconvolve it from the lake induced variations.

How to cite: Uthaman, M., Ermert, L., Ling, A., Junker, J., Ghisleni, C., and Obermann, A.: Temporal variation of ambient noise at the Grande Dixence reservoir recorded by a nodal deployment, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17811, https://doi.org/10.5194/egusphere-egu25-17811, 2025.

EGU25-18185 | Orals | EOS4.8

Advancing river plastic research through serendipity and stupidity 

Tim van Emmerik and the WUR-HWM River Plastic Team

Rivers play an important role in the global distribution of plastic pollution throughout the geosphere. Quantifying and understanding river plastic pollution is still an emerging field, which has advanced considerably thanks to broad efforts from science, practice, and society. Much progress in this field has been achieved through learning from failures, negative results, and unexpected outcomes. In this presentation we will provide several examples of serendipity and stupidity that has led to new insights, theories, methods, and completely new research lines. We will share what we learned from rivers flowing in the wrong direction, sensors that disappear, equipment blocked by invasive plants, and dealing with suspicious local authorities. Pushing the science sometimes requires an opportunistic approach, embracing surprises and chaos you may face along the way.

How to cite: van Emmerik, T. and the WUR-HWM River Plastic Team: Advancing river plastic research through serendipity and stupidity, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18185, https://doi.org/10.5194/egusphere-egu25-18185, 2025.

With the advent of parallel programming in the late 1990s. A port of the than available Max Planck Institutes for Meteorology spectral atmospheric model echam5 to MPI and OpenMP was done. For testing and validation of the hybrid parallelization a coherence algorithm was developed. The implementation has been incorporated into todays NWP and climate model ICON as well. The coherence algoritm consists of several stages: first one MPI rank is running the serial model against an n-task MPI parallelized model. During runtime the state vector is checked for binary-identity. If successfull a m-task MPI version can be compared to an m-task MPI version for high processor counts. The same schema can be used OpenMP parallelization. ONe MPI task runs the model serial using one OpenMP thread and a second MPI task runs k OpenMP threads. Again, the results are compared for binary-identity. As the testing needs to be done automatically, bit-identity is important for testing not necessarily for production.

The tesing revealed plenty of problems during the initial parallelization work of echam5 and showed constant appearing problems in the ICON development phase.

However, far in a couple of century long simulation the bit-identity was just by accident found to be broken: the search of the cause started!

How to cite: Kornblueh, L.: MPI and OpenMP coherence testing and vaildation: the hybris of testing non-deterministic model code, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18400, https://doi.org/10.5194/egusphere-egu25-18400, 2025.

EGU25-18981 | ECS | Posters on site | EOS4.8

Publishing BUGS: Insights from the Journal of Trial and Error 

Stefan Gaillard

Addressing positive publication bias and clearing out the file drawer has been at the core of the Journal of Trial and Error since its conception. Publishing the trial-and-error components of science is advantageous in numerous ways, as already pointed out in the description of this panel: errors can lead to unexpected insights and warning others about dead ends can prevent wasted time and other resources. Besides those advantages, publishing negative and null results facilitates conducting robust meta-analyses. In addition, predictive machine learning models benefit from training on data from all types of research rather than just data from studies with positive, exciting results; already researchers are reporting that models trained on published data are overly optimistic.

Besides publishing negative and null results as well as methodological failures, the Journal of Trial and Error couples each published study with a reflection article. The purpose of these reflection articles is to have a philosopher, sociologist or domain expert reflect on what exactly went wrong. This helps contextualize the failure, helping to pinpoint the systematic factors at play as well as helping the authors and other scientists to draw lessons from the reported research struggles which can be applied to improve future research.

Publishing failure brings with it some practical challenges: convincing authors to submit manuscripts detailing their trial-and-error; instructing peer reviewers on how to conduct peer review for the types of articles; differentiating between interesting … and uninformative, sloppy science; and determining the best formats to publish various failure-related outcomes in. Authors are still hesitant to publish their research struggles due to reputational concerns and time constraints. In addition, authors often fear that peer reviewers will be more critical of articles describing research failures compared to articles reporting positive results. To counteract this (perceived) tendency of peer reviewers to be more critical of research without positive results, we provide specific instructions to peer reviewers to only assess the quality of the study without taking into account the outcome. This then also ensures that we only publish research that adheres to the standards of the field rather than sloppy science. Whether submitted research provides informative insights is assed by the editor-in-chief and the handling editor.

Finally, we are constantly evaluating and innovating the types of articles we publish. Various types of errors and failures benefit from differing ways of reporting. For example, recently we introduced serendipity anecdotes, a format where scientists can anecdotally describe instances serendipity which occurred during their research. This format allows researchers to focus on the conditions which allowed for the serendipitous discovery rather than the research itself.    

How to cite: Gaillard, S.: Publishing BUGS: Insights from the Journal of Trial and Error, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18981, https://doi.org/10.5194/egusphere-egu25-18981, 2025.

It is common to perform two-dimensional simulations of mantle convection in spherical geometry. These have commonly been performed in axisymmetric geometry, i.e. (r, theta) coordinates, but subsequently we (Hernlund and Tackley, PEPI 2008) proposed using (r, phi) spherical annulus geometry and demonstrated its usefulness for low-viscosity-contrast calculations. 

When performing scaling studies in this geometry, however, strange results that did not match what is expected from Cartesian-geometry calculations were obtained when high-viscosity features (such as slabs) were present. It turns out that this is because the geometrical restriction forces deformation that is not present in 3 dimensions. Specifically, in a 2-D spherical approximation, a downwelling is forced to contract in the plane-perpendicular direction, requiring it to extend in the two in-plane directions. In other words, it is "squeezed" in the plane-perpendicular direction.  If the downwelling has a high viscosity, as a cold slab does, then it resists this forced deformation, sinking much more slowly than in three dimensions, in which it could sink with no deformation. This can cause unrealistic behaviour and scaling relationships for high viscosity contrasts. 

This problem can be solved by subtracting the geometrically-forced deformation ("squeezing") from the strain-rate tensor when calculating the stress tensor. Specifically, components of in-plane and plane-normal strain rate that are required by and proportional to the vertical (radial) velocity are subtracted, a procedure that is here termed "anti-squeeze". It is demonstrated here that this "anti-squeeze" correction results in sinking rates and scaling relationships that are similar to those in 3-D geometry whereas without it, abnormal and physically unrealistic results can be obtained for high viscosity contrasts. This correction has been used for 2-D geometries in the code StagYY (Tackley, PEPI 2008; Hernlund and Tackley, PEPI 2008) since 2010.

How to cite: Tackley, P.:  Adventures in Modelling Mantle Convection in a Two-Dimensional Spherical Annulus and Discovering the Need for "Anti-Squeeze”, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19890, https://doi.org/10.5194/egusphere-egu25-19890, 2025.

EGU25-20057 | Posters on site | EOS4.8

Some Perfectly Reasonable Ideas that Didn’t Work: Snow Hydrology 

Ross Woods

The science question: how can we use hydrological process knowledge to understand the timing and magnitude of seasonal streamflow in snow-influenced catchments.

What was known: in general, catchments with colder climates have later and larger seasonal streamflow peaks, because more snow tends to accumulate in colder catchments, and it melts later because the time when melt can occur is later in the year in colder climates. Numerical models with fine space and time resolution were able to resolve these phenomena, but there was no theory which directly linked long term climate to seasonal streamflow.

In 2009 I published a very simple deterministic theory of snow pack evolution. I tested it against snow observations at 6 locations in the western USA and it apparently worked well (although I later discovered that I'd been lucky).

In 2015 I used the snowmelt derived from this deterministic theory to predict timing and magnitude of seasonal streamflow. It did poorly, and revealed untested assumptions in my theory. I tried making the theory slightly more complicated by considering within-catchment variation in climate. This did not help.

In 2016 I created a stochastic version of the theory (a weakness identified in 2015), and then also considered the within-catchment variation in climate. It did better at reproducing measured snow storage, but did not help in understanding seasonal streamflow.

My next step will be to consider all forms of liquid water input, i.e. not just snowmelt but also rainfall.

What survived: I will continue to use the stochastic version of the theory as it is clearly an improvement. I will continue to examine whether within-catchment climate variability is important, but it seems unlikely after two negative results. But whether introducing liquid water input will be sufficient, who can say? I will also try to examine in more detail how it is that the finely-resolved numerical models can do an adequate job, but the theory cannot - it is in this gap that the answer probably lies.  However the models are very complicated, and it is not easy to get a good understanding of exactly what they are doing, even though we know which equations the are implementing.

 

How to cite: Woods, R.: Some Perfectly Reasonable Ideas that Didn’t Work: Snow Hydrology, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20057, https://doi.org/10.5194/egusphere-egu25-20057, 2025.

EGU25-20866 | ECS | Posters on site | EOS4.8

A case for open communication of bugs in climate models 

Jan Gärtner, Ulrike Proske, Nils Brüggemann, Oliver Gutjahr, Helmuth Haak, Dian Putrasahan, and Karl-Hermann Wieners

Climate models are not only numerical representations of scientific understanding but also human-written software, inherently subject to coding errors. While these errors may appear minor, they can have significant and unforeseen effects on the outcomes of complex, coupled models. Despite existing robust testing and documentation practices in many modeling centers, bugs broader implications are underexplored in the climate science literature.

We investigate a sea ice bug in the coupled atmosphere-ocean-sea ice model ICON, tracing its origin, effects, and implications. The bug stemmed from an incorrectly set logical flag, which caused the ocean to bypass friction from sea ice, leading to unrealistic surface velocities, especially in the presence of ocean eddies. We introduce a concise and visual approach to communicating bugs and conceptualize this case as part of a novel class of resolution-dependent bugs - long-standing bugs that emerge during the transition to high-resolution models, where kilometer-scale features are resolved.

By documenting this case, we highlight the broader relevance of addressing bugs and advocate for universal adoption of transparent bug documentation practices. This documentation complements the robust workflows already employed by many modeling centers and ensures lessons from individual cases benefit the wider climate modeling community.

How to cite: Gärtner, J., Proske, U., Brüggemann, N., Gutjahr, O., Haak, H., Putrasahan, D., and Wieners, K.-H.: A case for open communication of bugs in climate models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20866, https://doi.org/10.5194/egusphere-egu25-20866, 2025.

GI2 – Data networks and analysis

EGU25-275 | ECS | Orals | GI2.4

Application of Machine Learning Algorithms to Predict Rock Types Using Geochemical Data: A Case Study from the Obuasi Gold District, Ghana 

Abdullah Bello Muhammed, Emmanuel Daanoba Sunkari, and Abdul Wahab Basit

Artificial Intelligence and Machine Learning (AI/ML) are gaining increasing interest due to their capacity to increase precision and productivity in the current big data era. Machine learning has indicated its robustness in geosciences, particularly rock-type classification. Lithological classification in the traditional way has raised critical concerns and the need to curb the limitations it breeds, such as time consumption and subjective results. The gold mineralisation occurrence is structurally controlled in the Obuasi Gold district of Ghana. It exhibits complex patterns and relationships that may not be readily discernible through traditional methods, leading to missing out on discovering new resources or potential exploration targets. Consequently, this work attempts to create a predictive model by exploring the best machine-learning algorithms to predict rock types in the Obuasi Gold District using X-ray fluorescence (XRF) geochemical data. Here we established comparative predictive modelling using four supervised classification algorithms: Gradient Boosting (GBoost), Adaptive Boosting (AdaBoost), Support Vector Machine (SVM) and Random Forest (RF). The acquired XRF data was integrated with the model using the Google Collaboratory cloud-based platform. Results show that the performance evaluation of the models indicated SVM as the best algorithm for deployment with a Classification Accuracy (CA) of 0.902. Therefore, ML algorithms have been a great tool in rock-type classification, whereby SVM emerged as the best in the case of the Obuasi Gold District. However, it is encouraged to understand the geology of a particular area before employing the tool and the datasets must be balanced to yield good results and avoid model overfitting.

Keywords: Artificial intelligence; Machine learning algorithm; Support vector machine; Lithogeochemistry; Rock-type classification; Obuasi Gold District

How to cite: Muhammed, A. B., Sunkari, E. D., and Basit, A. W.: Application of Machine Learning Algorithms to Predict Rock Types Using Geochemical Data: A Case Study from the Obuasi Gold District, Ghana, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-275, https://doi.org/10.5194/egusphere-egu25-275, 2025.

Preserving clean water resources and efficiently treating wastewater is critical for ensuring human survival on Earth and in extraterrestrial environments. Major pollutants, including ammonium, heavy metals, industrial dyes, and chemicals, threaten limited clean water supplies and soil. Among the renowned absorbent materials, natural zeolite minerals have demonstrated their effectiveness for pollutant removal compared to clay minerals and synthetic equivalents like biochar, activated carbon, and MOFs, owing to their relatively extensive reserves and eco-friendly nature. Recently, investigating and optimizing pollutant removal rates from water without conducting laboratory experiments is getting more crucial, considering the time-consuming, expensive, and error-prone nature of laboratory testing due to human factors and potential calibration issues among the chosen analytical techniques.

This study aims to forecast the ammonium removal efficiency (% adsorption) and capacity (mg/g) of natural and modified zeolites from aqueous solutions using the regression ensemble LSBoost (MATLAB R2024b) machine learning (ML) algorithm, which is equivalent to XGBoost open-source library. A total of 527 experiments on 15 different zeolite compositions were gathered from a combination of 14 suitable moderately recent (≥ 2005) and highly referred studies to assess the performance of zeolite minerals on ammonium removal rates from aqueous solutions. The LSBoost algorithm achieved over 0.99 R2 fitting for training and overall, 0.95 R2 for prediction on the quarterly partitioned testing data for both efficiency and capacity. Throughout the improvement of the ML models using different random forest ML approaches, the number of predictors was successfully reduced to 8 based on importance rates among 31 different features in the initial dataset, with a negligible accuracy loss (<0.1 R2) on both training and testing. This research provides a valuable contribution to optimizing applicable experimental parameters in water treatment processes by effectively identifying the significance of predictors within a comprehensive data set. In addition to this, our model not only provides a robust predictive tool for optimizing zeolite performance in water treatment but also represents the first open-sourced web application in the literature to estimate the water treatment performance of zeolites.

How to cite: Akkaş, E., Ünal, B. C., and Ersoy, O.: AI-Based Prediction and Optimization of Ammonium Removal Efficiency and Capacity of Natural Zeolites Using LSBoost (XGBoost) for Sustainable Ecosystems, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-809, https://doi.org/10.5194/egusphere-egu25-809, 2025.

EGU25-882 | ECS | Orals | GI2.4

Assessment of a deep learning framework for time-lapse seismic monitoring 

Giovanni Pantaleo and Michele Pipan

In the context of CO₂ storage, cost-effective monitor methods are essential to ensure safe and long-term storage. This work explores the use of seismic time-lapse monitoring, combined with deep learning (DL) techniques, to assess potential leakage and migration pathways. The goal is to develop a cost-effective monitoring method while guaranteeing the safety of storage operations. To this end, we propose a Siamese Neural Network (SNN)-based framework to analyse shot gathers, designed to detect and localize changes within the storage complex. We aim to address the challenges of working with large seismic datasets, enabling the identification of significant events with high confidence, while avoiding the need for event-by-event processing. This framework can allow experts to rely on semi-automatic detections while ensuring human evaluation for interpreting and validating the results.

The proposed SNN architecture processes pairs of shot gather from baseline and monitor surveys in a cross-well configuration. It uses two identical neural networks with shared weights to encode the shot gathers into latent feature embeddings, which are then compared to identify similarities and detect changes. By transforming the data into a shared latent space, the model focuses on capturing relevant patterns while filtering out irrelevant variations, ensuring robust and accurate comparisons. When the SNN detects changes between the baseline and the monitor surveys, it highlights the regions where these changes occur. This approach is particularly effective for identifying subtle but important changes in seismic data, such as those caused by CO₂ migration, which alters the velocity and density of the subsurface. Even in noisy data, the SNN can detect these variations, thanks to its ability to learn features that are highly sensitive to small but meaningful changes. The SNN architecture is scalable and can be adaptable to various seismic monitoring tasks, requiring minimal preprocessing. The proposed framework harnesses the power of deep learning to provide insights into the dynamics of the storage complex, with a focus on identifying changes in time-lapse seismic data related to localized variations. The proposed migration detection tool offers a cost-effective and reliable solution to the modern challenges of gas storage monitoring. This study aims to enable operators to identify and address problems promptly, thereby minimising the impact of potential leakages.

How to cite: Pantaleo, G. and Pipan, M.: Assessment of a deep learning framework for time-lapse seismic monitoring, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-882, https://doi.org/10.5194/egusphere-egu25-882, 2025.

Joint inversion is an essential technique in potential field data processing. The current methodology largely relies on the geology model of anomalous bodies, especially for deep, complex structures. Inspired by the excellent nonlinear mapping capability of the image semantic segmentation model and the advantages of supervised learning, a regressive, end-to-end, encoder-decoder structural, convolutional neural network with a double-branch structure called PFInvNet(Potential Field Inversion Neural Network) is proposed for joint 3D  inversion of physical properties from gravity and magnetic data. Its input is a four-channel dataset consisting of gravity and magnetic anomalies and their vertical gradients, and its output is a 3D matrix representing the spatial distribution of the remnant density and the magnetic susceptibility, which are predicted independently through the double-branch structure of the decoders and then concatenated in the final layer. For network training, a large amount of precisely labeled sample is exceedingly demanding; thus, forward modeling becomes a prerequisite approach. Two discretized forward modeling algorithms for gravity and magnetic anomalies of 3D homogeneous arbitrary-shaped bodies based on surface integrals are deduced and verified with analytic solutions of the sphere model. Furthermore, the neural network needs to learn from the anomalies generated by various forms of abnormal bodies with different physical properties. Therefore, different sizes and quantities of cuboids are randomly distributed in the model space to simulate different forms of abnormal bodies. The label represents the combined spatial distribution of remanent density and magnetic susceptibility for the cuboids, encompassing both spatial location information and physical properties information. With the help of the Marching Cubes(MC) algorithm, the surface of the cuboids can be easily extracted and divided into a triangular surface mesh. The surface mesh is then used to calculate the gravity and magnetic anomalies synchronously through the forward modeling algorithms. The anomalies are concatenated in the channel direction as a sample. A set of optimal network parameters has been determined, including the weight initialization method, the gradient calculation methods, the loss function, the training hyperparameters, the regularization method, and the normalization method. The PFInvNet is trained with 500 and 10000 pairs of samples and labels, respectively. The analysis and comparison of training results prove that PFInvNet has two crucial features: one is that the branch structure enables independent prediction of magnetic susceptibility and remanent density; the other is efficient anti-overfitting ability and efficient solution-finding ability .The prediction error of small samples is very close to that of large samples and is also not obviously enhanced by the noise-contaminated data , demonstrating the strong generalization and robustness of the network. Finally, the network is tested with magnetic and gravity anomalies of the Victoria Land Basin in the western Ross Sea through transfer learning and retraining, and definite 3D distributions of apparent remnant density and apparent magnetic susceptibility have been obtained and can be checked with geological evidences.

How to cite: Jiang, W., Zhao, Y., Gao, J., Ge, S., and Xie, Z.: 3D property inversion of gravity and magnetic data based on a double branch regressive CNN trained by synchronous forward modeling :a case study of the Western Ross Sea, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1141, https://doi.org/10.5194/egusphere-egu25-1141, 2025.

EGU25-2156 | ECS | Orals | GI2.4

TOC Intelligent Prediction Model in Shale Reservoir: Integrating Data Enhancement with Empirically Driven Algorithm 

Yuzhen Hong, Shaogui Deng, Zhijun Li, and Zhoutuo Wei

Shale oil and shale gas are important unconventional resources. Organic matter serves as the primary source of shale oil and gas generation, and high TOC values typically indicate better oil and gas reservoir conditions and production. Therefore, an accurate TOC prediction model is conducive to low-cost evaluation of reservoir hydrocarbon potential and improvement of development efficiency. However, geochemical experimental measurements are costly, and the data obtained is discrete. It is unable to meet the requirements for fine-scale assessment of shale reservoirs. The multiple regression method and ΔlogR method, when directly applied to shale reservoirs, often result in significant errors. In this study, we propose a composite model for accurate TOC prediction in shale reservoirs based on data enhancement and empirically driven. We first address the issue of poorly characterized logging responses and discrete experimental data. The features and quantities of the dataset are enhanced by introducing reconstruction curves and generative adversarial networks (GAN). The validity of the synthesized data is then verified by plotting the data density. In the empirically-driven module, we optimize a density-gamma modified method on traditional ΔlogR method according to the characteristics of shale reservoirs. The modified ΔlogR method will be integrated into the GWO-SVR model as an empirically driven subject in the form of a fitness function. Above, a composite model with both empirical and data-driven components is constructed. We use the Dongying Depression in China as an example for model experiments. The composite model was generalized to wells X and Y. The R² (coefficient of determination) was 0.95 and 0.97, the RMSE (Root Mean Square Error) was 0.31 and 0.29, and the MAE (Mean Absolute Error) was less than 0.3, which indicated a high degree of consistency between the model predictions and the experimental values. Further controlled experiments revealed that the composite model predicted better than the ΔlogR method and the GWO-SVR model alone. Finally, we also performed SHAP interpretability analysis on the model. By revealing the decision-making mechanism inside the model, we verified the rationality of the empirical drive and enhanced the credibility of the model. This provides strong technical support and decision-making basis for the subsequent oil and gas exploration and development work.

How to cite: Hong, Y., Deng, S., Li, Z., and Wei, Z.: TOC Intelligent Prediction Model in Shale Reservoir: Integrating Data Enhancement with Empirically Driven Algorithm, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2156, https://doi.org/10.5194/egusphere-egu25-2156, 2025.

EGU25-2242 | Posters on site | GI2.4

A Conditional Neural Operator Approach for Resolution-Flexible and Parameter-Controlled Gravity Forward Modelling 

Ruiyuan Kang, Meixia Geng, Qingjie Yang, and Felix Vega

We present a novel approach to gravity forward modeling using conditional neural operators that establishes a forward generative model from the basin models and hyperparameters (reference basement depth, etc.) to gravity anomaly. Our methodology introduces an innovative adaptive embedding mechanism where scalar hyperparameters are first embedded into a 32-dimensional space and then adaptively expanded to match the dimensions of the basin depth model, enabling effective fusion with basin depth model data. Subsequently, Fourier Convolution Layers are employed to transform the fused data into gravity anomalies. The model demonstrates superior performance compared to existing convolutional neural networks on the test dataset, showcasing improved accuracy in capturing complex geological structures and their gravity responses. A key advantage of our architectural design is that it not only preserves the super-resolution capability of conventional neural operators but also enables controlled generation through different hyperparameters. This dual capability allows for both resolution-flexible modeling and parameter-controlled generation, while training on low-resolution data and producing high-resolution outputs, significantly reducing training data requirements and computational costs. The model's adaptive architecture effectively bridges the resolution gap between training and application scenarios, offering a practical solution for real-world geological surveys. Our results suggest that this approach could substantially improve the accessibility and applicability of gravity forward modeling in various geological settings, particularly in regions with limited high-resolution training data.

How to cite: Kang, R., Geng, M., Yang, Q., and Vega, F.: A Conditional Neural Operator Approach for Resolution-Flexible and Parameter-Controlled Gravity Forward Modelling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2242, https://doi.org/10.5194/egusphere-egu25-2242, 2025.

EGU25-2478 | Orals | GI2.4

International standards for responsible AI in disaster management 

Monique Kuglitsch and Elena Xoplaki

The combination of big data and AI/ML technologies shows tremendous promise within the domain of disaster management. So that benefits of AI/ML can be realized, and risks can be adverted, internationally agreed upon standards are an important mechanism. These can provide guidance on how to apply (and develop policy around) data collection and preprocessing, model training and evaluation, and operational implementation. In conjunction, they can cultivate interoperability and harmonization of AI-based systems. At the United Nations, the Global Initiative on Resilience to Natural Hazards through AI Solutions brings together experts from different disciplines (geosciences, disaster risk management, computer sciences) and sectors (government, research, NGO) to analyze use cases and lay the groundwork for such standards. Through proof-of-concept projects (e.g., HEU-funded MedEWSa), these standards can be further refined. Finally, through education and capacity building activities, the Global Initiative can help to democratize the responsible use of AI for this domain.

How to cite: Kuglitsch, M. and Xoplaki, E.: International standards for responsible AI in disaster management, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2478, https://doi.org/10.5194/egusphere-egu25-2478, 2025.

EGU25-4298 | ECS | Posters on site | GI2.4

Advances in the identification of geological discontinuities in boreholes with deep learning 

Rushan Wang, Martin Ziegler, Michele Volpi, and Andrea Manconi

Geological discontinuities significantly influence rock mass behaviour. Understanding the origin, setting, and properties of discontinuities is of major relevance, especially in boreholes. Traditionally, manual interpretation of borehole logs is done by geologists, a process that is time-consuming, costly, and subject to variability based on the interpreter's expertise. Recent advancements in artificial intelligence have made it feasible to use machine learning models and automatically detect and differentiate various features in digital images. In this study, we employ a state-of-the-art semantic segmentation model to tackle domain-specific challenges, enabling the identification of discontinuity types (e.g., natural faults, fault zones) and rock mass behaviour features (e.g., breakouts, induced cracks). We applied the SegFormer semantic segmentation model, which integrates a hierarchically structured transformer encoder with a multilayer perceptron (MLP). The borehole data used in this study was collected from the Mont Terri underground rock laboratory. Specifically, we labelled several high-resolution optical logs from one borehole and divided the dataset into training and testing subsets. The borehole considered is an experimental borehole designed to investigate the spatial and temporal evolution of damage around an underground opening in faulted clay shale. Our strategy achieved robust and accurate segmentation results on borehole images. Following segmentation, post-processing techniques were employed to extract critical information such as the total length of induced cracks and the total area of breakouts, as well as their locations and frequencies. The experimental results demonstrate high performance, with the pixel accuracy of 96 % in under three minutes for a 10-meter borehole. Our study lays the groundwork for future research by introducing a powerful tool for extracting geological structures and demonstrating the potential of AI models in geological analysis. By reducing processing time and increasing consistency in the identification, mapping, and classification of geological features, our approach can reveal spatial and temporal patterns associated with the evolution of rock masses.

How to cite: Wang, R., Ziegler, M., Volpi, M., and Manconi, A.: Advances in the identification of geological discontinuities in boreholes with deep learning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4298, https://doi.org/10.5194/egusphere-egu25-4298, 2025.

EGU25-4404 | ECS | Orals | GI2.4

AI-Enhanced Meteorological Data Retrieval Systems for Improved Forecast Operations 

Byeongyeon Kim, Hayan Shin, Areum Cho, Junsang Park, Hyesook Lee, ChaeHun Park, Jinkyung Joe, Jaegul Choo, and Minjoon Seo

Meteorological data are vast and complex, and their rapid and accurate retrieval is essential for forecasting operations. However, traditional systems have struggled with limited search accuracy and inefficient processing speeds, hindering effective forecast support. To address these challenges, this study developed an AI-based system capable of performing speech recognition, URL search, extreme value detection, and local forecast error analysis. In speech recognition, the Whisper-large model achieved a character error rate (CER) of 3.19%, with GPU memory usage reduced by 15.7% and inference time by 38.18%, enabling real-time processing and scalability in multi-GPU environments. The URL search systems translated natural language inputs into SQL queries and URLs, achieving a Mean Reciprocal Rank (MRR) of 0.92, thereby enhancing data retrieval precision. The extreme value detection systems utilized GPT-4-based template augmentation to expand training data by approximately 111%, significantly improving detection performance and search accuracy. For local forecast error analysis, a prototype chatbot was implemented using prompt engineering and a Text-to-SQL model, allowing for the automated identification of inconsistencies in local forecasts and streamlining the analysis process. These systems have substantially enhanced operational workflows across meteorological tasks, facilitating rapid data retrieval through voice commands, precise responses to complex queries, and real-time analytical support. Future research will focus on further refining these technologies to tackle a wider range of meteorological challenges and integrate them into global forecasting systems for enhanced accuracy and reliability.

How to cite: Kim, B., Shin, H., Cho, A., Park, J., Lee, H., Park, C., Joe, J., Choo, J., and Seo, M.: AI-Enhanced Meteorological Data Retrieval Systems for Improved Forecast Operations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4404, https://doi.org/10.5194/egusphere-egu25-4404, 2025.

EGU25-4699 | ECS | Orals | GI2.4

S-wave velocity prediction of shale reservoirs based on explainable physically-data driven model 

Zhijun Li, Shaogui Deng, and Yuzhen Hong

The shear wave (S-wave) velocity is a key basis for shale reservoir development, particularly for fracability evaluation. Additionally, S-wave velocity also plays a significant role in prestack seismic inversion and amplitude versus offset (AVO) analysis. However, the actual logging data often lack S-wave velocity data, so it is of significant importance for S-wave velocity prediction. We propose a rapid and precise prediction method for the S-wave velocity in shale reservoirs based on class activation maps (CAM) model combined with physically constrained two-dimensional Convolutional Neural Network (2D-CNN). High sensitivity curves related to S-wave velocity are selected as the foundation. Meanwhile, based on the petrophysical theory of pore medium, the petrophysical model of complex multi-mineral components is established. The dispersion effect is reduced to a certain extent and the results are used to constrain the model. The Adam optimization algorithm is used to construct a 2D-CNN model under the constraint of petrophysical model. The CAM is obtained by replacing the global average pooling (GAP) layer with a fully connected layer, which in turn leads to interpretable results. Then, the model is applied to wells A, B1, and B2 in the southern Songliao Basin. Afterwards, comparisons are made with unconstrained model and petrophysical model. The results show that the correlation coefficients and relative errors in the three test wells are 0.96 and 2.14%, 0.97 and 2.35%, and 0.97 and 2.9%, respectively. The higher prediction accuracy and generalization ability of the new method is confirmed. Finally, we present the defined C-factor as a means of evaluating the extent of concern regarding CAMs in regression problems. The C-factor confirms that the focus of 2D-CNN can be significantly enhanced by incorporating the petrophysical model, thereby imposing physical constraints on the 2D-CNN. In addition, we establish the SHAP model to assist in proving the importance of constraints.

Keywords: S-wave velocity prediction; Physically constrained 2D-CNN; Petrophysical model; Class activation mapping technique; Explainable results

How to cite: Li, Z., Deng, S., and Hong, Y.: S-wave velocity prediction of shale reservoirs based on explainable physically-data driven model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4699, https://doi.org/10.5194/egusphere-egu25-4699, 2025.

EGU25-7000 | ECS | Posters on site | GI2.4

Multivariate generative modelling of subsurface properties with diffusion models  

Roberto Miele and Niklas Linde

Accurate multivariate parametrization of subsurface properties is essential for subsurface characterization and inversion tasks. Deep generative models, such as variational autoencoders (VAEs) and generative adversarial networks (GANs), are known to efficiently parametrize complex facies patterns. Nonetheless, the inherent complexity of multivariate modeling poses significant limitations to their applicability when considering multiple subsurface properties simultaneously. Presently, diffusion models (DM) offer state-of-the-art performance and outperform GANs and VAEs in several tasks of image generation. In addition, training is much more stable compared to the training of GANs. In this work, we consider score-based DMs in multivariate geological modeling, specifically for the parametrization of categorical (facies) and continuous (acoustic impedance – I­P) distributions, focusing on a synthetic scenario of sand channel bodies in a shale background. We benchmark modeling performance against results obtained by GAN and VAE networks previously proposed in literature for multivariate modeling. As for the GAN and VAE models, the DM was trained with a training dataset of 3000 samples, consisting of facies realizations and co-located I­P geostatistical realizations. Overall, the trained DM shows significant improvements in modeling accuracy, for all evaluation metrics considered in this study, except for the sand-to-shale ratio, where the values are comparable to those of the GAN and VAE. In particular, the DM is 26% more accurate at reproducing the average (nonstationary) facies distribution and up to 90% more accurate at reproducing the IP marginal distributions for both sand and shale classes. Higher accuracy is also found in the reproduction of the facies-to-I­P joint distribution, whereas the spatial I­P distributions generated by the DM honour the two-point statistics of the training samples. The iterative generative process in DMs generally makes these networks more computationally demanding than VAEs and GANs. However, we demonstrate that with appropriate network design and training parametrization, the DM can generate realizations with significantly fewer sampling iterations while maintaining accuracy comparable to these benchmarking networks. Finally, since the proposed DM parametrizes the joint prior probability density function with a Gaussian latent space, it is straightforward to perform inversion. In addition to improved modeling accuracy, the mapping between the latent and image representations preserves a better topology than that of GANs, overcoming the well-known limitation of the latter for inference tasks, particularly for gradient-based inversion.

How to cite: Miele, R. and Linde, N.: Multivariate generative modelling of subsurface properties with diffusion models , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7000, https://doi.org/10.5194/egusphere-egu25-7000, 2025.

EGU25-9590 | Posters on site | GI2.4

Dynamic Time Warping algorithm: A geoscience aware AI for automatic interpretation in lithostratigraphy? Insights from an application to the Gulf of Corinth (Greece) 

Alina-Berenice Christ, Zahraa Hamieh, John Armitage, Renaud Divies, Sébastien Rohais, Luca Mattioni, and Antoine Bouziat

Stratigraphic correlation of well log data is a fundamental step in geosciences. It involves correlating stratigraphic units across multiple wells to build a comprehensive understanding of subsurface geology. Currently, stratigraphic correlation is predominantly performed “manually” by geoscientists. The process is labor-intensive and time-consuming, and interpretations may vary among interpreters due to differences in expertise, experience, and perspective.

Recent advancements in the application of the Dynamic Time Warping (DTW) algorithm have demonstrated its potential to automate and enhance the stratigraphic correlation of well logs. DTW can generate multiple correlation scenarios highlighting different interpretations of subsurface continuity. Thus, the aim of this work is to explore the potential of DTW as a supporting tool in the standard workflows of geoscientists and test it on well log data from IODP Expedition 381 from the Gulf of Corinth. We automatically correlate lithostratigraphic subunits within a 700 m thick stratigraphic unit across two wells, using Natural Gamma Ray (NGR) and Magnetic Susceptibility (MAGS) logs. We selected this dataset because it illustrates the evolution of geological interpretations over time. Between the first version of the IODP data interpretations and a second version published a few years later, significant differences in interpretation were proposed. These differences highlight the critical role of geological expertise in refining subsurface data interpretations and correlations.

The automatic correlations interpreted by DTW showed a minimal average absolute difference with the most recent and updated published correlation, making the human and the machine correlation almost identical. By applying DTW to this dataset, we demonstrate it would have been possible to identify discrepancies and challenges in the interpretations of subunits at the initial stages after data acquisition. This approach could have flagged potential issues even before the IODP data were made available on the public site. Such early identification highlights the potential of DTW as a valuable tool for providing immediate feedback and guiding more accurate stratigraphic interpretations faster.

While DTW significantly reduces the time required for the correlation phase, the time investment needed for data formatting upstream should not be underestimated. Future work on larger datasets will be crucial to better quantify and validate the overall time savings provided by DTW, as well as to optimize the preparatory steps to ensure efficiency in broader applications.

In conclusion, we show that DTW can offer innovative approaches to enhance geological investigations and speed up interpretations. More generally, we consider this work illustrates how data science methods can be leveraged to assist geologists in routine tasks, with our Corinth case study highlighting both the promises and current limitations of digital transformation in well correlations.  

How to cite: Christ, A.-B., Hamieh, Z., Armitage, J., Divies, R., Rohais, S., Mattioni, L., and Bouziat, A.: Dynamic Time Warping algorithm: A geoscience aware AI for automatic interpretation in lithostratigraphy? Insights from an application to the Gulf of Corinth (Greece), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9590, https://doi.org/10.5194/egusphere-egu25-9590, 2025.

EGU25-9671 | ECS | Orals | GI2.4

Kalpa: Empowering Artificial Intelligence-Driven Geospatial Analysis for Multidisciplinary Applications 

Sudhir Sukhbir, Satyam Pratap Singh, Utpal Singh, Mohit Kumar, and Tushar Goyal

In the age of big data, artificial intelligence (AI) is transforming Earth sciences by enabling efficient analysis and visualisation of complex datasets and fostering innovative approaches to solve age-old geoscientific challenges. Kalpa, a Python-based free and cross platform software, represents a pioneering step in this direction. Built with versatility at its core, Kalpa seamlessly integrates AI and machine learning workflows into geoscience applications, offering  customization through its Python plugin architecture. What sets Kalpa apart is its ease of use, even for non-experts. Its intuitive interface lowers the learning curve, enabling a broader audience—including researchers, professionals, and enthusiasts—to leverage advanced geospatial and AI tools without requiring extensive technical expertise.

Kalpa's capabilities span advanced 3D visualization, geospatial data processing, and machine learning model development. It supports global and regional raster and vector dataset visualisation and processing, allowing for interactive analysis in both geographic and cartesian coordinates. With tools to process satellite imagery, geological and geophysical data, uncrewed aerial vehicle (UAV) data, and digital geological maps, Kalpa caters to a wide range of applications, from mineral exploration to natural hazard forecasting. Its machine learning integration supports supervised and unsupervised algorithms for applications such as lithological mapping, mineral prospectivity mapping, land cover and land usage studies, agricultural productivity mapping and natural disaster management. In this study, we demonstrate Kalpa’s transformative potential through three case studies:

  • Lithological Mapping in Ladakh, India: Utilizing LANDSAT and SRTM data, we produced accurate lithological maps for this geologically complex region.
  • Copper Prospectivity Mapping in Northwest India: Combining remote sensing, geophysical, and geological data, Kalpa predicted copper mineralization zones, with all known deposits falling within areas of predicted probabilities exceeding 0.70.
  • Landslide Susceptibility Mapping in Uttarakhand, India: Using remote sensing datasets, Kalpa identified high-risk landslide zones, supporting disaster management efforts.

Kalpa’s user-friendly interface, robust machine learning integration, and publication-ready export capabilities position it as a powerful tool for advancing geoscience research and practical applications. By bridging the gap between domain expertise and cutting-edge AI methodologies, Kalpa empowers Earth scientists, environmental researchers, and GIS professionals to analyze, model, and predict with unprecedented efficiency and precision. This software marks a new frontier in the application of AI to Earth sciences, enabling multidisciplinary research and fostering innovative solutions to pressing geoscientific challenges.

How to cite: Sukhbir, S., Singh, S. P., Singh, U., Kumar, M., and Goyal, T.: Kalpa: Empowering Artificial Intelligence-Driven Geospatial Analysis for Multidisciplinary Applications, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9671, https://doi.org/10.5194/egusphere-egu25-9671, 2025.

EGU25-9968 | ECS | Posters on site | GI2.4

Advancing Landscape Archaeology with AI-driven insights from Airborne Laser Scanning data 

Nejc Coz, Žiga Kokalj, Susan Curran, Anthony Corns, Dragi Kocev, Ana Kostovska, Stephen Davis, and John O'Keeffe

Artificial intelligence (AI) is transforming landscape archaeology by enabling the automated analysis of high-resolution datasets, such as airborne laser scanning (ALS). The Automatic Detection of Archaeological Features (ADAF) tool is an example of the potential of AI to streamline the identification of subtle surface features and demonstrate their value in uncovering and understanding archaeological landscapes. By improving the detection of archaeological sites, the ADAF plays a crucial role in the research, management and preservation of cultural heritage.

ADAF uses advanced AI models, including convolutional neural networks (CNNs) for semantic segmentation and object detection, to detect features in ALS datasets. The tool has been trained on a large archive of ALS data from Ireland and processes visualised inputs to detect patterns indicative of archaeological structures. The workflow integrates pre-processing with the Relief Visualisation Toolbox, inference with trained AI models and post-processing to refine the results to ensure reliable outputs with minimal false positives.

Designed with accessibility in mind, ADAF features an intuitive user interface that removes the barriers traditionally associated with AI-driven analyses. Users can process ALS data and export GIS-compatible results without the need for specialised knowledge, making the tool suitable for a wide audience. This approach democratises the use of AI in landscape archaeology and extends its utility to professionals and researchers in the field.

Tests with Irish ALS datasets have shown that ADAF is able to detect both known and previously unrecognised archaeological features in the landscape, while enhancing the spatial accuracy of identified sites. By automating complex data analysis, ADAF underlines the efficiency, precision and scalability of AI in landscape archaeology. In addition, the tool contributes to the preservation of cultural heritage by identifying sites that would otherwise remain undiscovered and enabling their preservation and integration into cultural heritage management strategies.

ADAF represents a significant advance in the application of AI in landscape archaeology, providing a powerful and accessible solution for surface feature recognition. Its development underlines the transformative potential of AI to revolutionise the study and interpretation of archaeological landscapes.

How to cite: Coz, N., Kokalj, Ž., Curran, S., Corns, A., Kocev, D., Kostovska, A., Davis, S., and O'Keeffe, J.: Advancing Landscape Archaeology with AI-driven insights from Airborne Laser Scanning data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9968, https://doi.org/10.5194/egusphere-egu25-9968, 2025.

Borehole images (BHI) are crucial for resource exploration, providing detailed fracture analysis at millimeter-scale resolution. However, their interpretation is typically carried out manually, a process that is time-consuming, costly, and subject to significant uncertainty due to interpreter bias and variability. Current state-of-the-art AI methods for automated or semi-automated fracture analysis of BHI often rely on field data for training, using manual interpretations as labels. This approach inherently embeds both aleatoric (data-related) and epistemic (manual) uncertainties, which may undermine the reliability and adaptability of these methods. This study proposes an alternative, synthetic data-driven approach to train a set of two deep neural networks (DNNs) connected in sequence. These DNNs are designed to replicate the primary cognitive tasks involved in manual interpretation: the segmentation of the BHI to identify potential edge zones and the tracing of sinusoids over these edges to approximate their best-fitting 2D representation. By utilizing synthetic data, we are able to systematically assess the sensitivity of both networks and explore various training strategies, including curriculum learning (CL) and self-attention mechanisms. Our proposed solution is designed for post-hoc human-machine collaboration, where the model supports but does not replace human expertise. This framework enables the possibility of a multi-level uncertainty assessment—at the human, machine, and human-machine interface levels—opening the door to new ways of understanding and quantifying the sources of uncertainty in BHI analysis. Additionally, the synthetic data-driven approach ensures the generalizability and scalability of the method, as demonstrated by its successful application to low-resolution logging-while-drilling (LWD) and high-resolution fullbore formation microimager (FMI) datasets from multiple global locations. By combining advanced AI techniques with geoscientific knowledge, this study outlines a potential pathway toward more robust, ethical, and sustainable fracture analysis workflows. Beyond the traditional benefits of reduced cost and time, the approach may provide a scientifically grounded framework for exploring the benefits of human-machine collaboration and uncertainty quantification in geoscience practices. If adopted, this framework could significantly advance the field of BHI analysis, offering new tools for resource exploration in hydrocarbon and geothermal applications.

How to cite: Molossi, A., Roncoroni, G., and Pipan, M.: NeuroFit: a robust and scalable synthetic data-driven deep learning solution for automated borehole image analysis at LWD and wireline resolution, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10472, https://doi.org/10.5194/egusphere-egu25-10472, 2025.

EGU25-11754 | ECS | Orals | GI2.4

Exploring Pretraining Possibilities of Crop Classifiaction Models Using Large-Scale Sentinel-1 Datasets 

Mátyás Richter-Cserey, Máté Simon, Gabriel Magyar-Santen, Vivien Pacskó, and Dániel Kristóf

Since 2014, ESA Sentinel missions have been producing an ever-growing amount of data for Earth Observation. This creates the opportunity to monitor changes in high temporal and spatial resolution, however, interpreting this huge quantity of data is challenging. In recent years, the rapid advancement and widespread adoption of applied Artificial Intelligence (AI) methods made it feasible to create deep learning models for specific Earth Observation applications. Combining Sentinel datasets with the appropriate amount of ground truth, robust pre-trained models can be created and applied to produce good-quality thematic maps for different years and large areas. Due to responsibilities related to the European Union’s Common Agriculture Policy (CAP) and the motivation for regional yield estimation, crop classification is one of the most frequently studied remote sensing problems these days. Several papers investigate the possible methods to construct robust and generally functioning models to map the spatial distribution of crops as accurately as possible.

In this study, we present the development of a modular, pre-trained deep learning model designed specifically for crop type mapping. The model is tailored to classify the most prevalent crops in Hungary, including winter and autumn cereals, corn, sunflower, alfalfa, rapeseed, grasslands, and other significant types. For pre-training, we leverage country-wide Sentinel-1 Synthetic Aperture Radar (SAR) data such as Sigma Naught or polarimetric descriptors from H-A-alpha decomposition, collected during the 2021–2024 time period. This dataset comprises annual time series of Sentinel-1 pixels at a spatial resolution of 20 meters. Our approach builds upon prior findings that Sentinel-1-based crop type classification performs comparably to methods using Sentinel-2 optical data. However, Sentinel-1 has the added advantage of producing consistent and regular time series, as it is unaffected by atmospheric conditions such as cloud cover.

The proposed model employs a hybrid methodology integrating self-supervised and fully supervised learning paradigms. This modular architecture allows for seamless integration of task-specific classifiers, which can be fine-tuned using supervised learning to address both current and future classification requirements effectively. The fully supervised component is supported by an extensive ground truth dataset covering over 60% of Hungary’s total land area. This proprietary dataset is derived from the national agricultural subsidy database, providing detailed and accurate annotations. The abundance and quality of labeled data enable the construction of robust, highly generalizable models, ensuring reliable performance across diverse classification tasks. This methodology offers great potential to advance national-scale operational tasks, such as early land cover prediction and annual crop type mapping.

How to cite: Richter-Cserey, M., Simon, M., Magyar-Santen, G., Pacskó, V., and Kristóf, D.: Exploring Pretraining Possibilities of Crop Classifiaction Models Using Large-Scale Sentinel-1 Datasets, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11754, https://doi.org/10.5194/egusphere-egu25-11754, 2025.

EGU25-12065 | ECS | Orals | GI2.4

Calibration of the Hypoplastic Clay model with a deep neutral network 

Phuong Do and Tomas Kadlicek

Advanced constitutive models, here represented by the hypoplastic clay model, are powerful tools which provide engineers with reliable responses in various practical applications. However, the model calibration is not an easy task. Calibration of these models can be addressed with several approaches, which are generally distinguished as stochastic or deterministic approaches. In general, these approaches extract information from the experimental data and the subsequent optimisation process finds the best combination of parameters to fit the desired constraints. . The deterministic approach was integrated and combined in development of the online automated calibration tool ExCalibre. This paper presents a Machine Learning approach for automated calibration of the Hypoplastic Clay model. By using pairs of input experimental data and calibrated results performed by ExCalibre as training data, a Deep Neural Networks (DNNs) model is constructed to recognise how the experimental data can be used to derive the asymptotic state parameters such as the slope and the interception of the Normal Compression Line (NCL), or the critical friction angle, and the optimised stiffness parameters. The training and testing data comprise of In-house protocols and User-upload data over 3 years of launching the ExCalibre, and synthetic data with small distortion to prevent overfitting. Finally, investigations on how the DNNs model recognises the asymptotic patterns, as well as its calibration results will be presented.

How to cite: Do, P. and Kadlicek, T.: Calibration of the Hypoplastic Clay model with a deep neutral network, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12065, https://doi.org/10.5194/egusphere-egu25-12065, 2025.

EGU25-12242 | Posters on site | GI2.4

Automated Particle Size Distribution Estimation of Rock Avalanches using Deep Learning 

Ruoshen Lin, Michel Jaboyedoff, Marc-Henri Derron, and Tianxin Lu

Accurate estimation of Particle Size Distribution (PSD) in rock avalanche deposits is essential for understanding the fragmentation processes and spatial distribution characteristics during mass movement. However, traditional methods, such as physical sieving or visual field estimation, are time-consuming, labor-intensive, and impractical for large-scale field measurements. To address these limitations, this study presents an automated PSD estimation framework that combines UAV imagery and deep learning-based segmentation. A synthetic dataset was used to train the segmentation model, improving its robustness across different scenarios. Image resolution adjustments were applied to improve detection accuracy for small and overlapping particles. Additionally, Fourier analysis was utilized to reconstruct smooth and continuous particle contours, to effectively handle overlapping particles. The reconstructed 2D outlines were further used to estimate 3D particle volumes through the shape-volume model based on laboratory and literature data. Projection correction was applied to mitigate image distortions to ensure precise volume predictions. The proposed approach overcomes the limitations of traditional methods dealing with complex particle distributions in real field environments. The results demonstrate the effectiveness of the proposed method for large-scale particle detection and volume estimation, providing new insights into rock avalanche fragmentation dynamics.

Keywords: Rock avalanche; Particle size distribution (PSD); deep learning; UAV Imagery

How to cite: Lin, R., Jaboyedoff, M., Derron, M.-H., and Lu, T.: Automated Particle Size Distribution Estimation of Rock Avalanches using Deep Learning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12242, https://doi.org/10.5194/egusphere-egu25-12242, 2025.

EGU25-12675 | ECS | Orals | GI2.4

Automatic Detection of Cimiciato Defect in Hazelnuts Using Deep Learning and X-ray Radiography 

Antonio Gaetano Napolitano, Giacomo Mele, Laura Gargiulo, Matteo Giaccone, and Andrea Vitale

Hazelnuts are a significant crop, with global production exceeding 1.25 million tons by 2023 (INC, 2023). Quality is threatened by biotic agents, including insects causing the cimiciato defect. This defect, from insect bites during fruit growth, results in off-flavor, tissue alterations, and lipid oxidation (De Benedetta et al., 2023). Damage can be external or internal (hidden cimiciato). Industrial quality standards often exceed official regulations, making effective selection crucial. Traditional visual inspection is time-consuming and subjective. Non-destructive methods like NIR and NMR have potential but limited applicability. Deep Learning (DL) has revolutionized image classification, proving effective in agriculture, including disease and pest management (Mohanty et al., 2016; Dhaka et al., 2021; Meena et al., 2023). This study explores Deep Learning (DL) for automated detection of the cimiciato defect in hazelnuts using X-ray radiographs. Cimiciato, caused by insect feeding, degrades hazelnut quality, requiring product selection. Traditional methods are time-consuming and subjective. We propose a Convolutional Neural Network (CNN) model trained on X-ray images to classify hazelnuts as healthy or infected. Results demonstrate the model's effectiveness, offering a non-destructive, automated quality control solution.
Radiographs were acquired using a cone-beam micro-tomograph. Each hazelnut was positioned on a rotating stage. A CNN model was used for classification. CNNs effectively extract features from images. Convolutional layers apply filters to identify features; pooling layers reduce data dimensionality; fully connected layers combine features for classification. The Inception-ResNet-V2 architecture was chosen, combining Inception modules and residual connections (Szegedy et al., 2017). The model was trained (128 image batch size, 0.001 learning rate, 30 epochs), comparing SGD, ADAM, and RMSP optimizers. Images were pre-processed: resizing, pixel normalization, and data augmentation. 
The test dataset evaluated the trained network. SGD, ADAM, and RMSP yielded similar results. Confusion matrices visualize performance. ADAM performed best, but all achieved good results, especially for cimiciato detection. 

Keywords: Cimiciato defect, Hazelnut, Deep Learning, X-ray radiography, CNN

How to cite: Napolitano, A. G., Mele, G., Gargiulo, L., Giaccone, M., and Vitale, A.: Automatic Detection of Cimiciato Defect in Hazelnuts Using Deep Learning and X-ray Radiography, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12675, https://doi.org/10.5194/egusphere-egu25-12675, 2025.

EGU25-13315 | Posters on site | GI2.4

Harnessing AI and Decentralized Networks for Next-Generation Geophysical Forecasting 

Gabriel Moraga, Steven Hristopoulos, and Noah Pearson Kramer

Artificial Intelligence (AI) is revolutionizing geosciences, aligning perfectly with the themes of session GI2.4 by enabling the analysis of complex, multidimensional datasets and delivering actionable insights at unprecedented scales. This study presents two innovative AI-driven frameworks addressing critical challenges in soil moisture prediction and geomagnetic disturbance forecasting. Both approaches leverage decentralized networks to achieve scalability, foster collaboration, and enhance model performance through continuous refinement by a distributed community of contributors.

For soil moisture prediction, our multi-stream base model integrates data from Sentinel-2 (high-resolution spectral imagery), SMAP L4 (volumetric water content), ERA5 (meteorological variables), and SRTM (elevation data). The model predicts surface and rootzone soil moisture with six-hour lead times, achieving RMSE values of 0.1087 m³/m³ and 0.1183 m³/m³, respectively, across diverse Köppen-Geiger climate zones. By utilizing a decentralized network, contributors perform inference on 100 km² global regions, generating predictions evaluated against SMAP data using Root Mean Square Error (RMSE) and R² metrics. This system ensures robust model performance while addressing the spatial and temporal gaps inherent in traditional observational networks. These advances have significant implications for agriculture, hydrology, and climate modeling, enabling better water resource management, crop planning, and drought mitigation strategies. 

In geomagnetic disturbance forecasting, our GeoMagModel leverages Prophet, a time-series forecasting library, to predict the Disturbance Storm Time (Dst) index, a key indicator of geomagnetic activity. The model achieves an RMSE of 6.37 for December 2024 datasets, effectively capturing both trend shifts and weekly seasonality. The decentralized community enhances predictive accuracy by dynamically integrating historical and real-time Dst data, which is validated by benchmark predictions of the Kyoto World Data Center’s hourly records. This approach provides near-real-time forecasts critical for safeguarding power grids, satellite systems, and other infrastructure vulnerable to space weather events.

By integrating machine learning with decentralized computing and state-of-the-art data sources, these frameworks offer scalable solutions to longstanding challenges in geophysical monitoring. The decentralized network not only improves scalability but also incentivizes the geoscience community to refine baseline models, fostering innovation and enabling systems to outpace state-of-the-art benchmarks. The implications of this work extend beyond immediate applications, paving the way for hybrid models that combine AI-driven predictions with physical process-based simulations. This fusion has the potential to improve understanding and resilience in critical domains such as water resource planning, disaster mitigation, and space weather forecasting. By addressing the limitations of traditional observation systems and delivering actionable insights at scale, these AI-driven frameworks represent a paradigm shift in how we approach and solve complex geoscientific problems.

How to cite: Moraga, G., Hristopoulos, S., and Pearson Kramer, N.: Harnessing AI and Decentralized Networks for Next-Generation Geophysical Forecasting, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13315, https://doi.org/10.5194/egusphere-egu25-13315, 2025.

EGU25-15949 | ECS | Posters on site | GI2.4

Advanced Super-Resolution Techniques for Optical Payloads in Earth Observation: Combining Traditional and Deep Learning Methods 

Camilla De Martino, Vincenzo Della Corte, Laura Inno, Fabio Cozzolino, Giacomo Ruggiero, Vania Da Deppo, Paola Zuppella, Lama Moualla, and Sara Venafra

Small satellite platforms are increasingly used for Earth observation due to their cost-effectiveness and flexibility. However, their limited payload size often results in reduced spatial resolution of captured images. In our work, we address this challenge by proposing an advanced multi-image super-resolution (MISR) approach tailored for small satellite applications.

It integrates:

  • Sub-pixel image registration and on curvelet transform-based interpolation to preserve high-frequency details while reducing artifacts;
  • A novel hybrid method called SP-MISR (Subpixel Multi-Image Super-Resolution), which leverages Convolutional Neural Networks (CNNs) for local detail analysis and Transformers for global spatial relationships.

Our experimental results demonstrate that this combined approach  significantly improves image sharpness, preserves fine details, and reduces artifacts, outperforming traditional super-resolution techniques. Moreover, SP-MISR exhibits robustness in processing noisy and distorted images, making it particularly suitable for the constrained imaging systems of small satellites.

Future developments will focus on improving computational efficiency, reducing interpolation errors, and extending the method to multi-spectral imaging and interplanetary missions, by exploring explore pure deep learning techniques.

This work highlights the potential of integrating traditional and deep learning methodologies to enhance image quality, thus expanding the scientific and operational capabilities of small satellite missions.

How to cite: De Martino, C., Della Corte, V., Inno, L., Cozzolino, F., Ruggiero, G., Da Deppo, V., Zuppella, P., Moualla, L., and Venafra, S.: Advanced Super-Resolution Techniques for Optical Payloads in Earth Observation: Combining Traditional and Deep Learning Methods, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15949, https://doi.org/10.5194/egusphere-egu25-15949, 2025.

Soil carbonates are critical players in the global carbon cycle and have a profound influence on soil health and agricultural productivity. Their quantification is also central to carbon sequestration efforts, where accurate measurement of soil carbonates can inform strategies for reducing atmospheric CO2. However, conventional methods of carbonate analysis in soil---while effective---are often slow, costly, and labor-intensive (1).

In this study, we introduce Shifted Excitation Raman Difference Spectroscopy (SERDS) as a rapid, non-destructive alternative, further enhanced by advanced preprocessing techniques and machine learning algorithms. Specifically, we employ Asymmetric Least Squares (ALS) for background correction, Standard Normal Variate (SNV) for normalization, and Savitzky–Golay filtering for smoothing. Unlike conventional Raman spectroscopy, SERDS effectively eliminates background fluorescence and reduces overlapping peaks, resulting in clearer spectral signatures (2)

We employed Partial Least Squares Regression (PLSR) and eXtreme Gradient Boosting (XGBoost) to predict the inorganic carbon content from the carbonate vibrational modes in conventional Raman and SERDS spectra, benchmarked against total inorganic carbon (TIC) measurements from coulometric titration. Our results show that switching to dual-laser SERDS substantially boosted model performance. For PLSR, the coefficient of determination (R2) improved from 0.8 to 0.88 (an increase of about 10.5%), and the root-mean-square error (RMSE) declined from 0.29 to 0.22 (26% decrease). The XGBoost model exhibited an even greater increase, with R2 increasing from 0.63 to 0.93 (approximately 49% improvement) and RMSE dropping from 0.39 to 0.16 (59% reduction).

Figure 1: Left: All SERDS data of soil samples showing the main carbonate peak; Right: XGBoost model prediction of soil inorganic carbon using SERDS data.

These findings underscore the potential of SERDS to replace conventional methods for carbonate quantification, offering reduced cost, faster analysis, and essentially no sample preparation. Furthermore, by providing highly accurate carbonate measurements, this methodology can be pivotal for carbon sequestration assessments and large-scale soil management practices, helping to advance both environmental sustainability and agricultural productivity.

References:

1) Barra I, Haefele SM, Sakrabani R, Kebede F. Soil spectroscopy with the use of chemometrics, machine learning and pre-processing techniques in soil diagnosis: Recent advances–A review. TrAC Trends in Analytical Chemistry. 2021 Feb 1;135:116166.

2) Orlando A, Franceschini F, Muscas C, Pidkova S, Bartoli M, Rovere M, Tagliaferro A. A comprehensive review on Raman spectroscopy applications. Chemosensors. 2021 Sep 13;9(9):262.

How to cite: Poursorkh, Z., Solomatova, N., and Grant, E.: Quantifying Soil Inorganic Matter: Integrating Shifted Excitation Raman Difference Spectroscopy (SERDS) with Machine Learning for Enhanced Analysis of Carbonates, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16705, https://doi.org/10.5194/egusphere-egu25-16705, 2025.

Seismic exploration heavily relies on the accurate processing of seismic data, as high-quality reconstructed data is essential for reliable imaging and interpretation. In recent years, data-driven approaches have shown great promise in seismic data processing. However, supervised learning methods require large amounts of labeled data, while generative models, such as GANs, often encounter issues like mode collapse and instability. On the other hand, generative diffusion models, leveraging principles from nonequilibrium thermodynamics and Markov processes, have emerged as powerful tools for capturing complex data distributions.

Despite these advantages, Denoising Diffusion Probabilistic Models (DDPM) purely generate data distributions from the latent space with the reliance on random noise, making it inadequate for seismic data reconstruction where the goal is to accurately recover missing traces. Thus, DDPM is  lacks interpretability in seismic data restoration, and may disrupt the structured patterns crucial for interpolating seismic signals. Furthermore, we view the reverse process that starts from noise as unnecessary and inefficient for reconstruction task.

To address these challenges, we propose a novel Conditional Residual Diffusion Model (CRDM) that enhances both certainty and interpretability by incorporating residual diffusion and conditional constraints derived from observed seismic data (Fig.1). This approach better aligns with the inherent structure of seismic signals, enabling more accurate and interpretable reconstruction. The model is grounded in DDPM, with mathematical derivations for loss functions, conditional probability distributions, and reverse inference steps, ensuring both theoretical rigor and practical applicability.

Additionally, Our CRDM utilizes a shallow U-Net architecture featuring one down-sampling and one up-sampling layer integrated with Multi-Head Self-Attention (MHSA), which significantly enhances the model's efficiency and effectiveness. Experimental results (Fig.2) demonstrate that CRDM outperforms DDPM, denoising convolutional neural network (DnCNN), and fast projection onto convex sets (FPOCS), achieving a 15.1% improvement in reconstruction SNR and reducing computation time by 139 times compared to DDPM. Notably, CRDM achieves optimal results in a few diffusion steps, whereas DDPM typically requires thousands of steps.

The innovative approach generates data through residuals for determinism, while guiding the processing with noise for diversity. This not only enhances the interpretability and efficiency of seismic data reconstruction, but also positions the model as a promising tool for advancing data-driven seismic processing through flexible coefficient adjustment. Therefore, we believe this model has great potential for broader applications in geophysical data analysis, offering significant value in accurately depicting complex geological structures and providing more effective guidance for petroleum exploration.

Fig.1 The framework of CRDM. The model consists of two stage: (a) the training stage with forward diffusion process; (b) the sampling stage for seismic data reconstruction.

Fig.2 Reconstruction results and residuals of the 1994 BP seismic data with 50% irregular missing traces. (a) Complete data, reconstruction using (b) FPOCS (SNR=10.5dB), (c) DnCNN (SNR=15.6dB), (d) DDPM(SNR=18.4dB), (e) CRDM(SNR=21.2dB), and (f) observed seismic data with 50% missing traces. (g-j) display the residuals corresponding to reconstructions (b-e), respectively. The red box highlights a zoomed-in region, which is shown in detail in (k-t).

 

How to cite: Gong, X. and chen, S.: Enhancing Seismic Data Reconstruction with a Conditionally Constrained Residual Diffusion Model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16835, https://doi.org/10.5194/egusphere-egu25-16835, 2025.

Recent trends in climate change and global warming have amplified the occurrence of severe convective initiation (CI) and other extreme weather events, underscoring the importance of high-frequency remote sensing. Modern satellite constellations such as EUMETSAT, GOES, Himawari, and GK2A now offer global monitoring intervals of 10 minutes and regional updates as frequent as 1–2 minutes. However, these capabilities are not universally accessible—many developing countries lack in-orbit assets or historical high-frequency data archives.

This study presents a zero-shot video frame interpolation (VFI) approach to generate high-frequency (1–10 minute) satellite imagery from legacy or sparsely sampled observations. Leveraging a flexible Many-to-Many Splatting VFI model, our framework avoids domain-specific retraining while delivering reliable intermediate frames. We validate the method using overlapping data from the KMA GK2A (10-minute full-disk, 2-minute Asia-Pacific) and KMA COMS (3-hour full-disk, 15-minute Asia-Pacific) satellites over the period July 25, 2019, to March 31, 2020.

Our results indicate significant improvements in both PSNR and SSIM metrics, confirming the model’s efficacy in three critical applications:

  • Up-sampling Archived Geostationary Data

    • Enhancing the temporal resolution of older satellite imagery (e.g., COMS 30-minute or 3-hour intervals) to match or approximate modern satellite capabilities (e.g., GK2A 10-minute intervals). This harmonization facilitates unified climatology analyses spanning multiple generations of instruments.
  • Sensor-Error Correction and Gap Filling

    • Recovering missing or corrupted frames resulting from attitude adjustments, sensor calibrations, or malfunctions on geostationary satellites. Ensuring a continuous record provides more robust inputs to operational forecasting and climate assessments.
  • Delayed High-Frequency Observation Services

    • Enabling resource-constrained meteorological agencies to retrospectively produce and disseminate high-frequency satellite products (e.g., near 1-minute intervals) to improve nowcasting, risk assessment, and disaster preparedness.

Our preliminary findings show minimal computational overhead per inference step, making this cost-effective method feasible for near-real-time deployment and post-event analyses alike. By bridging temporal gaps in global satellite datasets, this technique supports advanced level-2 products such as cloud-tracking and convective-initiation alerts, thereby driving broader socioeconomic and scientific benefits in both developed and developing regions.

How to cite: Ryu, H. and Choi, Y.: Toward High-Frequency Satellite Observations in Data-Sparse Regions: A Zero-Shot Interpolation Framework for Missing and Historical Imagery, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17456, https://doi.org/10.5194/egusphere-egu25-17456, 2025.

EGU25-17957 | Posters on site | GI2.4

Fuzzy clustering of electrical and seismic data for the detection of geophysical targets 

Giorgio De Donno, Michele Cercato, Davide Melegari, Valeria Paoletti, Guido Penta de Peppo, and Ester Piegari

Tomographic methods, such as electrical resistivity tomography (ERT), induced polarization (IP) and seismic refraction tomography (SRT) are often effective for detecting geophysical targets in disparate real-world scenarios. However, a final reconstruction expressed only in terms of individual geophysical parameters (resistivity, chargeability, P-wave velocity) leaves room for ambiguity in complex sites exhibiting several transitions between layers or zones having different geophysical properties. In such cases, the sensitivity of the geophysical parameters for the various methods can differ significantly, so that a univocal interpretation based only on a visual comparison of the different models is often ineffective. To overcome these limits, in this work we present a machine learning-based quantitative approach for the detection of geophysical targets associated with both geological and anthropogenic scenarios. We integrate two-dimensional ERT, IP and SRT tomographic data with a soft clustering analysis by the Fuzzy C-Means (FCM) to obtain a final combined section, where each pixel is characterized by a cluster index and an associated membership value. The membership function of the Fuzzy C-Means is a good estimator of the accuracy of the subsurface reconstruction, as it ranges from 0 to 1, with 1 reflecting a high reliability of the clustering analysis. We apply this method to two case studies, related to the detection of leachate accumulation areas in a municipal solid waste landfill and to the bedrock characterization in a site prone to instability. In both cases, we detect the cluster associated with the geophysical targets of interest and our final sections are validated by a good agreement with the available direct information (boreholes and wells). The accuracy of the reconstruction is consistently high across most areas (membership values > 0.75), even though it is reduced in areas where the resolution of geophysical data is lower. Therefore, this approach may be a valuable automatic tool for optimizing the cost-effectiveness of projects where new constructions or remediation interventions have to be planned.

How to cite: De Donno, G., Cercato, M., Melegari, D., Paoletti, V., Penta de Peppo, G., and Piegari, E.: Fuzzy clustering of electrical and seismic data for the detection of geophysical targets, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17957, https://doi.org/10.5194/egusphere-egu25-17957, 2025.

EGU25-18082 | ECS | Orals | GI2.4

Integrating FDEM data with K-Means clustering for improved archaeological site identification 

Angelica Capozzoli, Valeria Paoletti, Federico Cella, Mauro La Manna, and Ester Piegari

The Frequency Domain Electromagnetic (FDEM) method is a cost-effective geophysical technique that simultaneously studies the electrical and magnetic properties of a medium, providing data as in-phase and out-of-phase components of the electromagnetic field. Although FDEM yields valuable insights, its results can be complex to interpret, and the two EM field components are normally only visually inspected to support findings from other techniques. This study aims to enhance FDEM data interpretation using an unsupervised learning technique. The proposed approach seeks to automate and expedite the interpretative phase. By applying the K-Means clustering algorithm, we divided the FDEM data into several clusters based on specific intervals of the in-phase and quadrature components, resulting in integrated maps of EM components. Combining these maps with geological and archaeological insights helped identifying areas of potential archaeological interest. This method was applied to the Torre Galli archaeological site in Calabria, Italy, known for its significance in Iron Age studies.

Based on comparisons with the findings of earlier excavations and results from a magnetic survey, the proposed procedure shows promise in improving the efficiency and accuracy of the FDEM method in identifying areas of archaeological interest. This suggests that automating the interpretation process could lead to a better cost management and time optimization in geophysical and archaeological studies.

How to cite: Capozzoli, A., Paoletti, V., Cella, F., La Manna, M., and Piegari, E.: Integrating FDEM data with K-Means clustering for improved archaeological site identification, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18082, https://doi.org/10.5194/egusphere-egu25-18082, 2025.

Artificial Intelligence (AI) is revolutionizing the field of geomorphology, offering a robust tool for objective and quantitative analyses. This pioneering study proposes an innovative framework based on Machine Learning clustering techniques, capable of classifying drainage patterns into multiple morphological classes. This work follows up on a related study in which an attempt at classifying 156 terrestrial and extraterrestrial (Mars and Titan) river networks was made. Rivers’ outlines are intrinsically noisy, difficult to isolate from the background, and can be ambiguous for the human eye. The previous works have been focused on accurately classifying patterns, using the expertise of morphologists, thus introducing a weak link, the human eye, in the chain. This time, a reliable, automatic, and scalable methodology has been obtained, leveraging computers’ precision, objectivity, and computational power. The HydroRIVERS dataset, a publicly available data bank containing vector data, was utilized in this study. All HydroRIVERS data layers are provided in a geographic projection (latitude/longitude), referenced to the WGS84 datum. Each data layer includes an attribute table with information on the morphometric characteristics of each river reach. The input parameters for the clustering models included morphometric features such as LENGTH_KM, DIS_AV_CMS, ORD_STRA, ORD_CLAS, and ORD_FLOW.
During a preliminary experiment, a local convexity test was conducted to determine the optimal number of clusters (k) to identify the best metric values. This test made sure that the number of clusters with the highest evaluation metric was selected, varying in a closed numeric interval. Each cluster corresponds to a specific river class. Significant results were obtained with k = 6, k = 8, k = 10, and k = 12. Subsequently, the K-Means algorithm was applied, grouping the dataset into distinct clusters based on the morphometric parameters. The results were remarkable, with 10 being the best value for k. The results indicate that the clustering algorithm is able to optimally separate the dataset, producing a high inter-cluster distance and a low intra-cluster distance. The dataset points along the features, as highlighted by the three principal components obtained by performing PCA on the final five-dimensional clustering resulting vector space, are well grouped in relatively small clusters, far away from each other. The next step involves using the centroids obtained from the analysis of the large dataset as a reference for classifying the 155 rivers. In general, the centroids obtained from this kind of Learning could be of great value to the scientific community, establishing a new and innovative way of discerning between different classes of rivers without having to manually analyze and inspect images. This approach promises efficient and accurate classification of both terrestrial and extraterrestrial drainage patterns.

How to cite: D'Aniello, M. and Donadio, C.: A novel approach using Machine Learning to objectively classify terrestrial and extraterrestrial river networks, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19838, https://doi.org/10.5194/egusphere-egu25-19838, 2025.

EGU25-20509 | Orals | GI2.4 | Highlight

Making Sense of AI: The Important Role of Education and Communication 

Luis Azevedo Rodrigues

The big developments in Artificial Intelligence (AI) generated a mixture of fascination and apprehension, echoing historical responses to unknown phenomena. Like how medieval European societies interpreted certain natural events and instruments as magical, AI is currently perceived by many as a “black box,” blurring the lines between advanced technology and mystical force. This phenomenon fosters misconceptions and uncertainties about AI’s actual mechanisms, benefits, and risks. Consequently, it underscores the urgent need for science communicators and science museums to adopt an active role in enhancing the general public’s AI literacy and in debunking some of its enigmatic traits.

By drawing parallels with the Middle Ages—when objects such as mirrors and magnetite were often attributed supernatural capabilities—modern AI tools LLMs or image and video generators are frequently viewed as possessing a “magical” principle. The public’s limited grasp of how AI processes inputs and produces outputs further intensifies this impression. The lack of transparency (or “black box” effect) in deep learning algorithms, combined with the ambiguity of human language, has been shown to fuel both wonder and anxiety.

Science museums and communicators should have an active role by offering educational programs that demystify AI through different demographic and social activities as well as promoting the public debate. These initiatives could clarify AI’s underlying mathematical and computational principles, highlight practical examples of AI-driven applications, and examine ethical considerations surrounding its deployment. Public understanding of AI’s capabilities and limitations is crucial not only to temper undue fears but also to encourage informed engagement with emerging technologies.

How to cite: Azevedo Rodrigues, L.: Making Sense of AI: The Important Role of Education and Communication, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20509, https://doi.org/10.5194/egusphere-egu25-20509, 2025.

EGU25-1280 | Posters on site | GI2.5

Atmospheric Dispersion Model for a Nuclear Accident using RAPS-K 

Kyung-Suk Suh, Kihyun Park, Byung-Il Min, Sora Kim, Yoomi Choi, Jiyoon Kim, Min-Chae Kim, Hyeonjeong KIm, and Kyeong-Ok Kim

The environmental and health effects of the transport and diffusion of pollutants released into the atmosphere and ocean due to a nuclear accident must be evaluated rapidly and accurately to ensure the safety of the surrounding population and ecosystem. Since the Fukushima accident in 2011, a web-based nuclear emergency support system named Radiological Accident Preparedness System in Korea (RAPS-K) has been developed to predict the dispersion of radioactive materials released into the environment and estimate dose assessment for humans. The system is composed of atmospheric dispersion, marine dispersion, and dose assessment models, along with a graphic user interface module. It can evaluate the dispersion patterns of radionuclides in the air and ocean, and the short-term and long-term radiological effects of a nuclear accident on humans. The atmospheric dispersion, marine dispersion, and dose assessment models have already been validated by model-to-model comparisons and measurements from the Chernobyl and Fukushima accidents. Especially, atmospheric dispersion model is connected with numerical weather forecast data produced by Korea Meteorological Administration (KMA) in real-time and the air conentrations are rapidly calculated in the system. Atmospheric dispersion model named LADAS(Lagrangian Atmospheric Dose Assessment System) was applied to evaluate the behavior of radioactive material released into the air for the hypothetical nuclear accident. RAPS-K is now operating through a web Graphic User Interface (GUI) on Linux OS. The developed system covers the Northeast Asian and worldwide regions in the event of a nuclear accident.

How to cite: Suh, K.-S., Park, K., Min, B.-I., Kim, S., Choi, Y., Kim, J., Kim, M.-C., KIm, H., and Kim, K.-O.: Atmospheric Dispersion Model for a Nuclear Accident using RAPS-K, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1280, https://doi.org/10.5194/egusphere-egu25-1280, 2025.

EGU25-2406 | ECS | Posters on site | GI2.5

Deep Neural Network for risk assessment via organ dose estimation in inhomogeneous radiation fields 

Yoomi Choi, Hyoungtaek Kim, Min Chae Kim, Sora Kim, Byung-Il Min, Jiyoon Kim, Kyung-Suk Suh, and Jungil Lee

When radiation exposure occurs, evaluating the radiation dose is necessary to assess the risk and implement appropriate protective measures. Typically, radiation workers use personal dosimeters, which conservatively calculate the effective dose based on measured values. However, in scenarios involving potential high radiation exposure, emergency response tasks, or accidental exposure, precise dose evaluation is crucial. Conventional methods estimate human dose from dosimeter readings by applying dosimeter-to-human dose conversion factors under the assumption of a parallel radiation field, but this can introduce significant errors when the radiation field is inhomogeneous.
In this study, Deep Neural Networks (DNN) was applied to rapidly estimate absorbed doses to humans and dose conversion factors in inhomogeneous radiation fields. It was assumed that the radiation field can be described by the location and energy distribution of point sources, and the basic exposure scenario was set to external exposure by a standing adult male from a point source. Through GEANT4-based Monte Carlo simulations, absorbed doses to radiation-sensitive organs and whole-body were calculated, and conversion factors between chest-worn dosimeters and organ doses were determined.
Due to significant skewness in dose data, statistical techniques that transform the data to approximate a normal distribution, such as log transformation and Box-Cox transformation, to facilitate more effective training. The transformed dataset was divided into training, validation, and test sets. Optimization of model hyperparameters was performed using training and validation data and optimized model was trained. The model's predictive performance was verified by evaluating its relative error rate in predicting test data compared to ground truth values. The prediction results demonstrated an acceptable relative error rate, factoring in the uncertainty inherent in simulation-derived data. The results of this study are expected to provide a foundation for easily and quickly assessing the predicted risk to the human body when radiation exposure occurs in an unexpected inhomogeneous source distribution situation. This will help to quickly determine follow-up measures.

How to cite: Choi, Y., Kim, H., Kim, M. C., Kim, S., Min, B.-I., Kim, J., Suh, K.-S., and Lee, J.: Deep Neural Network for risk assessment via organ dose estimation in inhomogeneous radiation fields, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2406, https://doi.org/10.5194/egusphere-egu25-2406, 2025.

EGU25-2649 | Posters on site | GI2.5

Improvement of a model for estimating radionuclide concentration in marine organisms in a marine environment exposure dose assessment model 

Sora Kim, Kyung-Suk Suh, Dong-Kwon Keum, Byung-Il Min, Yoomi Choi, Jiyoon Kim, Minchae Kim, Hyeon-Jeong Kim, and Kihyun Park

We recently developed a marine environment exposure dose assessment model to evaluate the radiological doses to the public following marine radiological accidents. The following six exposure pathways were considered: external exposure through beach activity, swimming, and boating and internal exposure through inhalation via sea spray, ingestion of seawater during swimming and ingestion of seafood. A model for estimating radionuclide concentration in marine organisms in the present dose assessment model was developed based on the equilibrium model, taking into account realistic aspects related to food intake and data availability related to model input variables. However, when the equilibrium model was applied in the early phase of an accident in which the radionuclide concentration changes significantly, there is a possibility that the evaluation result of nuclide concentration in marine organisms could be overestimated, so a dynamic marine foodchain model was added to the equilibrium model-based marine dose assessment module so that it can be selectively applied according to the purpose of the assessment. When applying the dynamic model, the limitations of the model to the uncertainty about the input variables and assessment results due to the lack of available data must be considered. The dynamic model considered three groups of seafood (fish, invertebrate, seaweed), as in the equilibrium model. The model contains  compartments for water, sediment, and marine organism groups. The radioactivity transfer for compartments is dynamically modeled by a first-order differential equation using rate constant. Radioactive decay is considered in all compartments. To the next step, it is planning to develop a module that can evaluate the public exposure doses by linking the dose assessment model with the marine dispersion model, and apply it to the case study for calculating the public exposure following hypothetical marine radiological accidents.

How to cite: Kim, S., Suh, K.-S., Keum, D.-K., Min, B.-I., Choi, Y., Kim, J., Kim, M., Kim, H.-J., and Park, K.: Improvement of a model for estimating radionuclide concentration in marine organisms in a marine environment exposure dose assessment model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2649, https://doi.org/10.5194/egusphere-egu25-2649, 2025.

In this study, the FLEXPART atmospheric transport model was used to simulate the atmospheric transport of Cs-137 following the Fukushima NPP accident in March 2011, using the source term estimation described in [1]. The simulation results were compared with airborne concentration measurements conducted in Japan and globally. It was shown that FLEXPART results as compared to Fukushima are highly sensitive to assumptions regarding size distribution of the radioactivity in the source. Based on our study, 'conventional' assumptions regarding the mean aerodynamic diameter (MAD) of particles, which are typically reported in the range of 0.2 to 0.7 μm in various studies, yielded reasonable agreement between simulated and observed concentrations within Japan. However, at greater distances from the source (e.g., across Eurasia), our results showed that the calculated concentrations were significantly overestimated. As discussed in our study, the size distribution of particles in the plume evolves over time. Therefore, measurements of AMAD conducted in Europe [2], which report a similar range of AMAD values, may not be representative enough to determine the initial AMAD at the source. To address this, we curve-fitted the observed size distribution of emitted particles measured in Japan shortly after the accident, as presented in [3]. This approach resulted in the following estimates for the size distribution: AMAD ≈ 2.5 μm and geometric standard deviation (GSD) ≈ 1.8. Simulations conducted with these updated size distribution parameters showed significant improvement in the agreement between calculated and observed airborne concentrations, as compared to using conventional assumptions.

References

  • 1. Terada H, Nagai H., Tsuduki K., et al. (2020) Refinement of source term and atmospheric dispersion simulations of radionuclides during the Fukushima Daiichi Nuclear Power Station accident, Journal of Environmental Radioactivity, Volume 213,106104, https://doi.org/10.1016/j.jenvrad.2019.106104
  • 2. Masson O., Ringer W., Malá H., et al. (2013) Size Distributions of Airborne Radionuclides from the Fukushima Nuclear Accident at Several Places in Europe. Environmental Science & Technology 47 (19), 10995-11003 DOI: 10.1021/es401973c
  • 3. Miyamoto Y., Yasuda K., Magara M., (2014) Size distribution of radioactive particles collected at Tokai, Japan 6 days after the nuclear accident, Journal of Environmental Radioactivity (132) 1-7, https://doi.org/10.1016/j.jenvrad.2014.01.010

How to cite: Kim, K. O., Kovalets, I., and Park, C.-W.: Evaluation of the parameters of size distribution of emitted aerosols for simulation of radionuclides atmospheric transport following Fukushima accident using FLEXPART model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2670, https://doi.org/10.5194/egusphere-egu25-2670, 2025.

EGU25-2671 | Posters on site | GI2.5

Development of the POSEIDON-GM–box-based radioactivity transport model for the global ocean: preliminary results of Cs-137 and Sr-90 distributions due to global fallout 

Kyung Tae Jung, Roman Bezhenar, Vladimir Maderich, Yulia Bezhenar, and Hanna Kim

According to the World Nuclear Association, the capacity of nuclear power plants around the world is growing steadily. In detail, about 60 reactors are under construction among which 29 reactors are to be launched by 2025 with 19 reactors located on the coast. This increases the risk of radioactive contamination of ocean waters in the case of potential nuclear accidents. Rapid growth of NPPs amount around the world requires the development of the global model that can simulate the release of radioactive materials from any NPP and assess its impact on the adjacent local/regional seas and global ocean. The compartment model POSEIDON with the new global system of boxes could be such a model which simulates transport of a wide range of radionuclides in the marine environment including marine food chains and calculates doses to humans from seafood consumption. Also, the model operates with both atmospheric and direct releases of radionuclides to the marine environment.

A new global system of boxes for the POSEIDON-GM (Global Model) has been developed which consists of 437 boxes of variable sizes. Most ocean boxes have 4 vertical layers in the water column: first surface layer with a depth of 30 m, second layer between 30 and 200 m depth, third layer between 200 and 1000 m depth, and fourth layer below 1000 m. Boxes with an average depth of less than 1000 m have fewer vertical layers depending on their depth. Water fluxes between boxes were calculated from the Global Ocean Physical Multi-Year product by Copernicus Marine Environment Monitoring Service, which contains monthly mean circulation data averaged for 1993-2016.

Annual depositions of 137Cs and 90Sr in each box of the POSEIDON-GM due to the global fallout have been calculated using data of deposition density from UNSCEAR for the 1945-1987 period with extrapolation for the 1988-2020 period. The transport of 137Cs and 90Sr entered the World Ocean due to global fallout has been simulated by POSEIDON-GM. Calculated concentrations of both radionuclides in water have been compared with measurement data from the MARIS database for the Southern Hemisphere, where the global fallout was the dominant source of radioactive contamination.

The next stage of the POSEIDON-GM development will include consideration of other sources of radioactive contamination, such as local sources from nuclear weapon tests, releases from nuclear reprocessing plants, sources due to Fukushima and Chornobyl nuclear accidents, etc. The model results will be compared with measurement data for concentrations of radionuclides in water and from different trophic levels of marine organisms from around the World Ocean. 

How to cite: Jung, . T., Bezhenar, R., Maderich, V., Bezhenar, Y., and Kim, H.: Development of the POSEIDON-GM–box-based radioactivity transport model for the global ocean: preliminary results of Cs-137 and Sr-90 distributions due to global fallout, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2671, https://doi.org/10.5194/egusphere-egu25-2671, 2025.

Since the mid-20th century, exposure to radioactive materials has occurred through various sources, such as nuclear tests, nuclear safety incidents, and releases from reprocessing plants. These materials have undergone global fallout and deposition through ocean-atmosphere circulation. This study aims to calculate the global spatial distribution of radioactive fallout on the Earth's surface based on observational data (fallout database), assuming wet deposition processes, and to evaluate temporal changes. The results will be utilized in a global climate model (GCM), Geophysical Fluid Dynamics Laboratory Earth System Model Version 4 (GFDL-ESM4), to better understand the patterns of deposition. Through this approach, we aim to estimate the extent of radioactive diffusion into the atmosphere and ocean and the subsequent accumulation in biological resources. Furthermore, this study investigates to assess how early 21st-century climate change may influence the global spatial variations of radioactive fallout and deposition.

How to cite: Seung-Hwon, H. and Hyung-Gyu, L.: Study of fallout distribution based on the wet deposition of major radiochemical species and application on the global climate model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2690, https://doi.org/10.5194/egusphere-egu25-2690, 2025.

Radioactive cesium-bearing microparticles (CsMPs) were insoluble glassy matrixes derived from Fukushima Daiichi Nuclear Power Plant accident. CsMPs have greater radioactive cesium (Cs) concentration per unit mass than other particles adsorbing Cs such as clay and organic particles (i.e., particulate Cs). In addition, the size of CsMPs was about a few µm. CsMPs may move around the environment as in the case of particulate Cs. Therefore, there is a concern for an internal exposure when CsMPs may enter the living organisms. Furthermore, previous studies have shown that CsMPs may attach to soil and crops, and locally increase Cs concentration of them. On the other hand, the difference of particulate Cs and CsMPs is Cs desorption from those particles. For particulate Cs, some Cs may electrically adsorb onto clay planar site and functional groups, therefore, their Cs may be exchanged with other cations, desorbed, and adsorbed by the crop through the roots. However, Cs in the CsMPs is included in in soluble grassy matrixes. In other words, it is considered that Cs in the CsMPs may be difficult for crops to absorb. Transfer factor (TF) is used to evaluate transfer of Cs from soils to crops. However, the conventional TF is a simple ratio of Cs concentrations between soils and crops. This suggests that conventional TF may not be able to accurately assess Cs transfer from soils to crops, since Cs in the soils contains a mixture of Cs with different crop availability. Since there are many contaminated forest areas in Fukushim, it is necessary to evaluate secondary contamination due to the inflow of Cs and CsMPs from these areas into farmland after decontamination.

In this study, we investigated the changes of Cs and CsMPs deposition in the paddy field in the first year of resumption of farming after the accident. Furthermore, we evaluate the contribution of CsMPs on particulate Cs to grasp the impact of CsMPs on TF of brown rice.

As a result, the accumulation of Cs and CsMPs increased in the entire field of this study in the period from plowing to harvest. The deposition of Cs per unit area increased in the center and the four corners of the paddy field other than inlet and outlet. This may be due to the deposition of suspended matter in areas with relatively litte water movement. On the other hand, there was no clear trend for CsMPs deposition in the paddy filed. This is because CsMPs were only detected in some of the soil samples, and the amounts varied depending on the soil. The Cs concentration in brown rice was less than 100 Bq kg-1-FW in all samples. This indicated that safe rice could be produced on this study site after decontamination. Furthermore, there was no significant difference between TF values with and without the contribution of CsMPs to Cs concentration in the soil. This suggested that there was no problem to evaluate TF using conventional methods for the paddy filed in Fukushima Prefecture.

How to cite: Tatsuno, T., Nihei, N., and Yoshimura, K.: The impact of radioactive cesium-bearing microparticles on Cs transfer factor of brown rice on the paddy field in the first year of resumption of farming, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3130, https://doi.org/10.5194/egusphere-egu25-3130, 2025.

EGU25-3386 | Posters on site | GI2.5

Record of the Fukushima nuclear accident in unsaturated soil water and the fate of nuclear contamination 

Tomoko Ohta, Keith Fifield, László Palcus, Stephen Tims, Stefan Pavetich, Hiroyuki Matsuzaki, Daisuke Tsumune, and Yasunori Mahara

The 3H and 36Cl radionuclides, released during the Fukushima nuclear accident in 2011, contaminated forested environments. However, the opportunity to periodically observe these radionuclides was lost due to the catastrophic conditions caused by the earthquake and tsunami associated with the accident. The concentrations of these released nuclides in precipitation and their fates are critical when considering the effects of internal exposure. Given that 3H and 36Cl are reliable hydrological tracers, records of their continuous depositional flux within unsaturated soil layers could provide valuable insights into the contamination levels during the initial years after the accident. Such records are indispensable for understanding the extent of contamination. Using a borehole drilled in 2014 at Koriyama, 60 km from the accident site, we reconstructed the deposition record of atmospheric 3H and 36Cl following the accident. The contributions of 3H and 36Cl from the accident were determined to be 1.4 × 1013 and 2.0 × 1012 atoms m−2, respectively, at this site. Unlike approaches based on radionuclide migration analysis, the 3H and 36Cl concentrations in precipitation during the approximately six weeks following the accident were accurately recovered (607 Bq/L and 4.74 × 1010 atoms/L, respectively) by analyzing the depositional flux in the unsaturated soil column from depths of 0 m to 4.25 m. Both the 3H and 36Cl concentration profiles were reassessed at the site in 2016. By that time, both soluble radionuclides had mostly been flushed out of the unsaturated soil zone due to rainfall over the 5.6 years since the accident. Although 3H concentrations in the unsaturated soil water and shallow groundwater had returned to less than 6 tritium units (TU), the 36Cl concentration had not yet returned to the natural cosmogenic background deposition level. In contrast, 129I was primarily found in the litter layer and the soil near the ground surface.

How to cite: Ohta, T., Fifield, K., Palcus, L., Tims, S., Pavetich, S., Matsuzaki, H., Tsumune, D., and Mahara, Y.: Record of the Fukushima nuclear accident in unsaturated soil water and the fate of nuclear contamination, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3386, https://doi.org/10.5194/egusphere-egu25-3386, 2025.

The world has experienced three major nuclear accidents (Chernobyl, Three Mile Island, and Fukushima). We have accumulated a vast amount of data from those accidents as well as from less severe nuclear accidents and incidents tracked in the nuclear industry. It is time for us to develop an open knowledge base that gathers and shares nuclear accident-related data and enables users to utilize those data to prevent future nuclear accidents and implement effective remediation measures when an accident occurs. However, nuclear-related data have peculiar challenges when it comes to understanding and organizing the data because of the behavior of radioisotopes. Having examined the nuclear accident literature, we identified four data axes that are important to organize nuclear accident data systemically. Those axes are: (1) historical time flow vs. nuclear decay (logarithmic radioactive decay), (2) temporal extent affected by radioactive decay vs. spatial extent affected by environmental processes, (3) contamination vs. non-contamination (background) comparison for which a comparison method is decided upon (1) and (2), and (4) radioactivity vs. dose (health risk inflicted on organisms) as a result of exposure to radioactivity. These four axes need to be considered in every step related to nuclear accidents.

For example, when a nuclear accident occurs, the first step is to assess the level of radioactive contamination in the nearby environment. Distinguishing the accident-derived radioactivity from the background radioactivity [axis 3] is crucial to implementing evacuation and remediation procedures and assessing health risks [axis 4]. However, comparing accident-driven radioactivity against the background activity is not straightforward. Identifying a proper background location and collecting a sample involves spatial and temporal considerations [axis 1, 2], such as sampling distance, direction, depth, sampling timing, sampling frequency, etc. So far, a data organization scheme for nuclear accidents has not been established despite the vast amount of accident/incident data accumulated and the possible severe implications of nuclear accidents to society.

We propose ontology as a tool that addresses the peculiar nature of nuclear data and systematically organizes the knowledge we have acquired on nuclear accidents. Ontology originated as a metaphysical study in the field of philosophy to study the properties and relations of all involved entities. With the help of ontology, we provide formal definitions of the entities within the nuclear accident knowledge domain and connect those entities with logical rules. In this study, as the first step of nuclear accident ontology building, we present an ontology-based conceptual model on background comparison for environmental radioactivity utilizing a well-established Basic Formal Ontology (BFO) for upper-level ontology and several ontology models that have been developed in the sub-fields of the nuclear and energy industries. The rule-based entity structure based on ontology will contribute to building a comprehensive knowledge base for nuclear accidents. Our aim is to build a knowledge base adaptable to machine learning that will shorten the time needed for nuclear accident data search and provide insights into the best practices to minimize the adverse effects on humans and the environment from nuclear accidents.

How to cite: Yasumiishi, M. and Bittner, T.: Developing Ontology-Based Nuclear Accident Knowledge Base Part 1: Spatiotemporal Considerations in Background Comparison, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5199, https://doi.org/10.5194/egusphere-egu25-5199, 2025.

EGU25-7764 | Posters on site | GI2.5

Analysis of the Impact of Precipitation on Tritium Concentrations Based on Nuclear Facility Operation Data 

Juyeol Yun, Jinhyung Lee, and Jong-Myoung Lim

Tritium is a radioactive substance released into the environment through air and water systems during nuclear facility operation, potentially affecting ecosystems. Understanding its concentration variations is essential. This study analyzed tritium concentrations measured in air (unit: Bq/m³) and rainwater (unit: Bq/L) from 2011 to 2022 to evaluate the reliability of sampling methods for atmospheric and precipitation samples. A multi-faceted analysis was conducted using variables such as precipitation, release rates, and seasonal factors. The results showed that increased precipitation led to decreased tritium concentrations in rainwater at all locations, with significant dilution effects observed in northern and western monitoring points (approximately -0.0309 Bq/L and -0.0301 Bq/L per 1mm precipitation increase, respectively). Tritium concentrations in the air also tended to decrease with increasing precipitation, although the magnitude of variation was smaller compared to rainwater. A statistically significant correlation between increased precipitation and decreased air tritium concentrations was observed at the eastern monitoring point (P < 0.01). Comparing tritium concentrations across seasons under similar precipitation conditions revealed no significant differences in most cases; however, slightly higher concentrations were found in winter. This may be related to specific factors such as temperature conditions or emission patterns during winter. This study quantitatively confirmed the environmental behavior of tritium and its dilution effect by precipitation, providing crucial baseline data for the long-term management of radioactive substances around nuclear facilities and contributing to the evaluation of sampling methods' reliability.

How to cite: Yun, J., Lee, J., and Lim, J.-M.: Analysis of the Impact of Precipitation on Tritium Concentrations Based on Nuclear Facility Operation Data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7764, https://doi.org/10.5194/egusphere-egu25-7764, 2025.

EGU25-8294 | Posters on site | GI2.5

Sedimentation areas along the Fukushima coast for Cs-bearing microparticles from the Lagrangian particle tracking 

Roman Bezhenar, Hyoe Takata, Daisuke Tsumune, Vladimir Maderich, and Yutaka Tateda

13 years after the Fukushima nuclear accident, the coastal area in front of the Fukushima Dai-ichi Nuclear Power Plant remains contaminated. First, it relates to the bottom sediments, which were contaminated with Cs-137 during the accidental and post-accidental releases. Additional contamination of bottom sediments could be caused by river runoff of Cs-bearing microparticles, which were formed in the initial phase of the accident, dispersed in the atmosphere, and fell into the watershed of nearby rivers. Cesium may be preserved in such particles for a long time due to its insoluble characteristics. River runoff carries suspended particles along with Cs-bearing microparticles to the coastal areas of the ocean, especially during heavy rains.

In the study, we applied the Lagrangian particle tracking model Parcels to identify places of potential deposition of such Cs-bearing microparticles in the Fukushima coastal area. As input data we used

  • 3D circulation data from the detailed ROMS-based ocean circulation model customized to the Fukushima coast for the period 2013-2016;
  • Estimates of released Cs-bearing microparticles from rivers during heavy rains in selected period;
  • Estimates of microparticles’ sizes define the vertical velocity of their falling in the water column.

Lagrangian particles simulated the transport of Cs-bearing microparticles, which were released from the Abakuma River mouth, by the coastal currents taking into account Stokes settling velocity. Maximums in the distribution of such particles on the bottom identified areas with possible accumulation of Cs-bearing microparticles in the coastal area after heavy rains. Distributions for different particles’ sizes obtained in simulations were analyzed.

How to cite: Bezhenar, R., Takata, H., Tsumune, D., Maderich, V., and Tateda, Y.: Sedimentation areas along the Fukushima coast for Cs-bearing microparticles from the Lagrangian particle tracking, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8294, https://doi.org/10.5194/egusphere-egu25-8294, 2025.

EGU25-10014 | Posters on site | GI2.5

Lagrangian pathways of 137Cs released from multiple sources in the Arctic Ocean 

Igor Brovchenko, Vladimir Maderich, Clara Lambin, and Vazira Martazinova

The Arctic Ocean and the North Pacific are the main reservoirs of anthropogenic radionuclides introduced in the past 80 years. The Lagrangian particle tracking approach was applied to the Arctic oceans to study the pathways of 137Cs contamination from point sources representing the locations of solid radioactive waste in the bays of the Novaya Zemlya archipelago and in the Kara Sea. The model includes radioactive decay and the interaction of dissolved radionuclides with suspended and bottom sediments. Lagrangian model uses accurate approach for simulating the absorption-desorption processes and novel algorithm for the bottom boundary conditions. As input for the model, the 3D hydrodynamic fields from NEMO model simulation with 10 km horizontal resolution and 121 vertical layers were used. 3D velocity fields along with vertical velocity and vertical turbulent mixing coefficient were used from NEMO simulation for 38 years from 1980 to 2018. Suspended sediment concentration fields were reconstructed using the 1D SEDTRANS05 sediment transport model in each grid node.

A set of potential scenarios of radioactive release were considered to analyse the most probable pathways of contamination. In each simulation, 1M of particles was used and individual trajectories were stored. The maps of visitation probability were built to show pathways of radioactivity contamination in the Arctic Ocean from the selected sources.

How to cite: Brovchenko, I., Maderich, V., Lambin, C., and Martazinova, V.: Lagrangian pathways of 137Cs released from multiple sources in the Arctic Ocean, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10014, https://doi.org/10.5194/egusphere-egu25-10014, 2025.

EGU25-10714 | ECS | Posters on site | GI2.5 | Highlight

 Predicting soil Radiocaesium uptake and dynamics using Mid-Infrared Spectroscopy (MIRS) 

Jumpei Iwai, Gerd Dercon, Magdeline Vlasimsky, Franck Albinet, Hayato Maruyama, and Takuro Shinano

The Radiocaesium (¹³⁷Cs) released as a result of past and potential nuclear accidents is of great concern for agriculture because of the relatively long half-life and easy absorption by plants. A countermeasure is the use of potassium fertilizers, but the relationship between transferability from soil to crop and exchangeable potassium (Ex K) varies depending on the soil. Previous studies have suggested that exchangeable ¹³⁷Cs (Ex ¹³⁷Cs) and the solid/liquid distribution coefficient (Kd) can be important factors explaining the variability of the ¹³⁷Cs dynamic in soil. However, the methods to measure these soil parameters are not suitable for adequate emergency deployment and preparedness because they are expensive and time consuming.

Mid-infrared spectroscopy (MIRS) has been shown to predict soil parameters more quickly and cost-effectively. However, the prediction of Cs parameters (Ex ¹³⁷Cs, Kd) using MIRS has not yet been evaluated. This study aims to evaluate whether MIRS can predict Cs-related parameters such as Kd, Ex 137Cs/Total 137Cs, and other parameters that may influence on the behavior of 137Cs in the soil, such as total carbon (soil total C).

The 1,682 samples were collected in Fukushima Prefecture, Japan from 2013 to 2020, most of them are Andosols. Each soil property (soil total C, Ex 137Cs/Total 137Cs ) was obtained from the monitoring data of MAFF and NARO. As for Kd for 133Cs, 176 samples were measured at Hokkaido University using ICP-MS. Each sample was dried at 37°C for at least one night and then sieved to less than 0.2 mm before measurement. The spectra data was obtained with four replicates in each soil sample using MIRS. To date, a total of 1,419 samples have been analyzed and their properties predicted using partial least squares regression (PLSR).

The PLSR models provided a relatively high accuracy for the prediction of soil total C, where the R2 (coefficient of determination) was 0.9±0.01. However, low accuracy was observed in the prediction of Kd for 133Cs, where the R2 was 0.46±0.06, which was attributed to the low concentration of the data and the limited number of samples. On the other hand, the result of Ex 137Cs/Total 137Cs showed relatively higher value then Kd for 133Cs, where the R2 was 0.56±0.04. Variable importance on projection Ex 137Cs/ Total 137Cs suggests that wavelength range related to clay mineralogy, quartz, and organic matter are influential in the estimation of Ex 137Cs/Total 137Cs.

 To further evaluate the potential for MIRS for rapid and affordable prediction of Radiocaesium risks, additional samples will be analyzed to improve the representativeness of the model and broaden the dataset, and more modeling techniques (Cubist, Support Vector Machine, etc) will be applied.

How to cite: Iwai, J., Dercon, G., Vlasimsky, M., Albinet, F., Maruyama, H., and Shinano, T.:  Predicting soil Radiocaesium uptake and dynamics using Mid-Infrared Spectroscopy (MIRS), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10714, https://doi.org/10.5194/egusphere-egu25-10714, 2025.

EGU25-14589 | Orals | GI2.5

Understanding H-3/Cs-137 Behavior to Track Dispersion Sources in Fukushima’s Marine Environment 

Nimish Sudhir Godse, Daisuke Tsumune, Hiroaki Kato, and Yuichi Onda

Thirteen years have passed since the accident at the Fukushima Daiichi Nuclear Power Plant, but the levels of Cs-137 and H-3 near the power plant have not returned to the levels they were at before the accident. In addition, the levels of Cs-137 and H-3 near the power plant continue to be higher than in other areas of the sea. This suggests a persistent leakage from the power plant or the surrounding sea area. However, the mechanism of the leakage is unknown. As the estimated rate of leakage outside the port is higher than the estimated rate of leakage inside the port, it is also possible that the leakage is not via the port.

The ratio of radioactive material concentration does not change in seawater over a short period of time, so it is useful for estimating the source of leakage. Here, we focused on the ratio of H-3 and Cs-137 and analyzed the data.

After 2016, the concentration of Cs-137 near the power plant has hardly decreased.

The concentration of Cs-137 and H-3 is high in the port area and low outside the port area. However, the H-3/Cs-137 ratio is small in the port area and large outside the port area. This suggests that the concentration of Cs-137 and H-3 in the port area does not necessarily affect the concentration outside the port area, and there is a possibility that there is another source.

The H-3/Cs-137 ratio fluctuates greatly over time. This may be due to the presence of multiple sources with different H-3/Cs-137 ratios, or it may be a sampling issue due to large fluctuations in concentration over time and space.

We have now started analyzing the H-3/Cs-137 ratio in nearby river water and groundwater and will discuss the relationship between these at the time of the presentation.

How to cite: Godse, N. S., Tsumune, D., Kato, H., and Onda, Y.: Understanding H-3/Cs-137 Behavior to Track Dispersion Sources in Fukushima’s Marine Environment, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14589, https://doi.org/10.5194/egusphere-egu25-14589, 2025.

EGU25-14834 | Posters on site | GI2.5

Simulation of the impact assessment of the discharge of ALPS treated water into the ocean 

Daisuke Tsumune, Takaki Tsubono, Kazuhiro Misumi, Tomomi Okamura, Hiroshi Abe, Hiroaki Kato, and Yuichi Onda

As part of the decommissioning work at the Fukushima Daiichi Nuclear Power Plant, the discharge of ALPS-treated water began in August 2023. ALPS-treated water contains not only H-3, but also other nuclides, albeit at extremely low concentrations. ALPS-treated water is treated so that the total of the concentration ratios of the 30 target nuclides is less than 1, and then diluted so that the H-3 concentration is less than 1500 Bq/L before being discharged. Prior to discharge, a radiation impact assessment was carried out by TEPCO. This assessment used a marine dispersion model that had been verified using observation results for Cs-137 that had leaked out as a result of the Fukushima Daiichi Nuclear Power Plant accident.

The ocean dispersion model was a 1 km x 1 km ROMS model with a variable mesh that was refined to 200 m x 200 m in the vicinity. It was driven by meteorological reanalysis data from the Japan Meteorological Agency, and data assimilation was performed using JCOPE2M ocean reanalysis data to reproduce the Kuroshio and mesoscale eddies.

In this assessment, a H-3 concentration of 0.1 Bq/L was used as the background concentration from atmospheric nuclear testing. However, a concentration of 1 Bq/L of H-3 was observed even before the release, and this is thought to be due to the influence of the supply from the power plant site or surrounding areas, or from rivers. After taking into account the influence of these background concentrations, the results of the model simulations were verified against the results of the monitoring of H-3 concentrations. Because the rate of release of the ALPS processed water was small, the range of influence of the monitoring of H-3 concentrations was limited, but the verification results were consistent. It is necessary to determine the average distribution by continuing to monitor in the future.

How to cite: Tsumune, D., Tsubono, T., Misumi, K., Okamura, T., Abe, H., Kato, H., and Onda, Y.: Simulation of the impact assessment of the discharge of ALPS treated water into the ocean, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14834, https://doi.org/10.5194/egusphere-egu25-14834, 2025.

EGU25-14888 | Orals | GI2.5

Field-Based Modeling of Cesium-137 Adsorption/Desorption Reactions in Fukushima River bottom Sediment 

Yuichi Onda, Naoyuki Wada, Yasunori Igarashi, and Jim Smith

The 2011 Fukushima Daiichi Nuclear Power Plant (FDNPP) accident released significant amounts of radioactive Cesium-137 (137Cs). Both dissolved and suspended forms of 137Cs contribute to river runoff. Although the Ministry of the Environment has monitored 137Cs in Fukushima river-bottom sediments since 2011, identifying long-term trends is challenging. Existing adsorption/desorption models focus on ideal lab conditions and lack real-world field data. This study uses long-term monitoring data to examine changes in 137Cs concentration in river sediments. Sediment samples were collected every four months, while river water and suspended sediment were sampled quarterly. The model simulates adsorption/desorption reactions between river water and sediments, incorporating fast and slow reaction sites. By adjusting reaction rates, measured and modeled 137Cs concentrations were optimized. Results show 137Cs concentrations in particle-size-corrected sediments aligned with suspended forms within a year. An increase in 137Cs concentration at 45 sites was observed, a phenomenon not seen in dissolved or suspended forms. The distribution coefficient (Kd) of river bottom sediments fluctuated significantly in the first three years. Slow adsorption dominated 137Cs accumulation within six months, while its effect on suspended concentrations was negligible. These findings highlight that slow adsorption/desorption processes are critical for the long-term behavior of 137Cs in river-bottom sediments.

How to cite: Onda, Y., Wada, N., Igarashi, Y., and Smith, J.: Field-Based Modeling of Cesium-137 Adsorption/Desorption Reactions in Fukushima River bottom Sediment, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14888, https://doi.org/10.5194/egusphere-egu25-14888, 2025.

EGU25-14889 | Posters on site | GI2.5

Long-term trends in 137Cs concentrations in rivers across Europe originating from Chornobyl 

Yasunori Igarashi, Yuichi Onda, and Jim Smith

Large-scale nuclear accidents may contaminate large areas of land with long-lived radionuclides such as 137Cs. Rivers are important pathways for transporting these radionuclides from upstream to downstream. The 137Cs concentration released during the Chornobyl nuclear accident has been shown to decrease over time. Previous studies also have shown that the concentration of 137Cs in rivers is influenced by competing ions, hydrological processes, the amount of adsorption sites on suspended particles, and the land cover of the catchment. However, comparative studies between rivers are limited, and the factors that determine the variation in 137Cs concentrations in rivers remain unclear. In this study, we collected time-series measurements of 137Cs from nine major rivers across Europe, each from different regions and countries affected by varying environmental conditions. We also characterized the properties of each river’s catchment, including land cover, water chemistry, and hydrological characteristics. By linking the 137Cs concentration data with these catchment attributes, we aimed to identify the most significant factors influencing 137Cs transport. Our findings reveal a quantitative relationship between the transport of 137Cs and the catchment characteristics, highlighting key factors that control radionuclide behavior in rivers. These results can be used for long-term predictions of radionuclide transport in rivers, which is crucial for risk assessment and management in regions affected by nuclear accidents.

How to cite: Igarashi, Y., Onda, Y., and Smith, J.: Long-term trends in 137Cs concentrations in rivers across Europe originating from Chornobyl, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14889, https://doi.org/10.5194/egusphere-egu25-14889, 2025.

EGU25-14919 | ECS | Orals | GI2.5

Elucidation and modeling of the effects of forest management on air dose rates 

Yusei Uehara, Yuichi Onda, Junko Takahashi, Miyu Nakanishi, Yupan Zhang, and Shiori Takamura

The Fukushima Daiichi Nuclear Power Plant accident, triggered by the Great East Japan Earthquake on March 11, 2011, caused large-scale radioactive contamination across terrestrial areas. Among the released radionuclides, Cesium-137 remains a significant source of radiation due to its long half-life, resulting in persistently high ambient dose rates in contaminated forests. To reduce these dose rates, forest thinning is being implemented as a radiation countermeasure. However, its effectiveness and the specific mechanisms through which thinning influences dose rates remain unclear. This study focuses on the relationship between forest thinning, throughfall, soil moisture, and ambient dose rates. Previous research has shown that rainfall temporarily reduces dose rates by increasing soil moisture, which attenuates gamma radiation from Cesium-137 in the soil. Building on these findings, we investigated the impact of thinning on rainfall reaching the forest floor and its subsequent effect on dose rates. Field studies were conducted at two sites, Iitoi and Fuyuzumi, located approximately 40 km northwest of the FDNPP. Thinning was implemented from October to December 2022, and monitoring devices were installed in April 2024. Results show that thinning increases throughfall and soil moisture, reducing dose rates over time. Soil moisture in thinned plots rose from 33.1% to 35.0%, while control plots decreased from 28.6% to 25.5%. Correspondingly, ambient dose rates dropped from 0.9 μSv/h to 0.75 μSv/h in thinned plots, compared to 0.85 μSv/h in control plots. Based on these observations, we developed a long-term predictive model to estimate ambient dose rates from rainfall and soil moisture data, providing a generalized framework for assessing the long-term impact of forest management on radiation levels in contaminated areas. 

How to cite: Uehara, Y., Onda, Y., Takahashi, J., Nakanishi, M., Zhang, Y., and Takamura, S.: Elucidation and modeling of the effects of forest management on air dose rates, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14919, https://doi.org/10.5194/egusphere-egu25-14919, 2025.

EGU25-16740 | Posters on site | GI2.5

Long term variations of 137Cs and 90Sr distribution in the Sea of Japan  

Yayoi Inomata, Daisuke Tsumune, and Katsumi Hirose

Anthropogenic radionuclides were released into the world's oceans as a result of large-scale weapons testing in the late 1950s and early 1960s. These anthropogenic radionuclides have long lifetimes and are still present in the oceans today. The behavior of long-lived radionuclides is useful for seawater circulation in the global ocean.

In this study, we focus on the spatiotemporal variations in the 137Cs and 90Sr activity concentrations in the surface seawater and vertical distributions. Most of data were included into the database, Historical Artificial radioactivity database in Marine environment, Global integrated version 2021 (Inomata and Aoyama, 2023). The ratio of 137Cs to 90Sr from large-scale nuclear tests was reported by Harley et al. (1965) to be 1.45. These ratios were in agreement with the average value of the ratio found in open ocean seawater (1.43±0.70) (Bowen et al., 1974). However, the ratios analysed in the present study did not always consistent with the reported values. This may be due to the different behaviour of 90Sr and 137Cs, e.g. 137Cs is mainly present in the dissolved form, whereas 90Sr is incorporated into particles in seawater. Furthermore, the 90Sr/137Cs ratio may be closely related to seawater circulation. However, as data on 90Sr are very scarce compared to 137Cs, detailed analysis of long-term variations in the 137Cs/90Sr ratio is limited to the North Pacific Ocean and its marginal sea.

The results showed that the 137Cs/90Sr ratio varied in the northern North Pacific and adjacent waters (northern North Pacific Ocean (NNPO), western North Pacific Ocean (WNPO), Sea of Japan (SOJ), Sea of Okhotsk (OKH) and East China Sea (ECS)). The apparent half-life (Tap) of 90Sr in ECS were longer than those in other area. Considering that a longer Tap indicates a larger inflow into the area and a shorter Tap indicates a lower inflow, it can be assumed that the OKH has sources of 137Cs and 90Sr. At some SOJ stations, the ratio of 90Sr/137Cs was large at depths greater than 2000 m. Furthermore, inventories of 137Cs and 90Sr have increased since 1990 at the SOJ stations. The increase in inventories may be attributed to the dumping of radioactive material.

How to cite: Inomata, Y., Tsumune, D., and Hirose, K.: Long term variations of 137Cs and 90Sr distribution in the Sea of Japan , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16740, https://doi.org/10.5194/egusphere-egu25-16740, 2025.

Understanding the transport of 137Cs released during the Fukushima accident remains challenging, as existing source terms fail to adequately capture the critical emissions leading to the high-deposition zone. For the problem, this study presents an objective inverse reconstruction method that uses total deposition and atmospheric concentration data. The deposition data is used to extract the a-priori emissions by novel identifying the critical temporal formation process of these depositions in high-deposition areas, with the help of the WRF-Chem model, and deriving the corresponding emissions. This deposition-based prior was then fused with the concentration data within an inversion framework, compensating the spatiotemporal information of incomplete data and ensuring the continuity feature of the emissions.

The reconstructed source term reveals two prominent emission peaks on March 15, 2011, occurring between 10:00-11:00 and 14:00-15:00. These peaks align with in-situ pressure measurements and accident analysis, suggesting that they were caused by pressure drops in the primary containment vessels of Units 3 and 2, respectively. This finding provides an explanation for the observation of spherical 137Cs particles, likely formed through the condensation of vaporized or liquefied substances. The reconstructed source term also independently validates the widely adopted reverse estimation results by JAEA.

Simulations based on the reconstructed source term show significantly better agreement with various observational data than simulations using other source terms. The two-peak emission pattern accounts for the high-deposition areas, supporting the accuracy of the reconstruction. Furthermore, the proposed method outperforms traditional direct fusion approaches that combine deposition and atmospheric concentration data, which often fail to provide satisfactory results due to insufficient temporal information in deposition observations.

This new method offers a powerful tool for multi-observation fusion, providing a more accurate extraction of temporal information from total depositions. It represents a significant advancement in source term reconstruction, especially for complex nuclear accidents. The approach has broader implications for understanding the transport of short-lived radionuclides, with potential applications in iodine emission reconstruction, thyroid dose evaluation, and improving future environmental assessments in nuclear accident scenarios.

 

How to cite: Fang, S., Dong, X., Xu, Y., and Hu, H.: Uncovering the Key 137Cs Emission Sources Contributing to High-Deposition Zones After the Fukushima Accident, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20921, https://doi.org/10.5194/egusphere-egu25-20921, 2025.

EGU25-240 | ECS | Posters on site | ESSI3.1

Leveraging Machine Learning and Remote Sensing for Water Quality Analysis in Lake Ranco, Southern Chile 

Lien Rodríguez-López, Lisandra Bravo Alvarez, Iongel Duran Llacer, David Ruíz-Guirola, Samuel Montejo-Sánchez, Rebeca Martínez-Retureta, Luc Bourel, Frederic Frappart, and Roberto Urrutia

This study examines the dynamics of limnological parameters of a South American lake located in southern Chile with the objective of predicting chlorophyll-a levels, which are a key indicator of algal biomass and water quality, by integrating combined remote sensing and machine learning techniques. Employing four advanced machine learning models, the research focuses on the estimation of chlorophyll-a concentrations at three sampling stations within Lake Ranco. The data span from 1987 to 2020 and are used in three different cases: using only in situ data (Case 1), using in situ and meteorological data (Case 2), using in situ, and meteorological and satellite data from Landsat and Sentinel missions (Case 3). In all cases, each machine learning model shows robust performance, with promising results in predicting chlorophyll-a concentrations. Among these models, LSTM stands out as the most effective, with the best metrics in the estimation, the best performance was Case 1, with R2 = 0.89, an RSME of 0.32 μg/L, an MAE 1.25 μg/L and an MSE 0.25 (μg/L)2, consistently outperforming the others according to the static metrics used for validation. This finding underscores the effectiveness of LSTM in capturing the complex temporal relationships inherent in the dataset. However, increasing the dataset in Case 3 shows a better performance of TCNs (R2 = 0.96; MSE = 0.33 (μg/L)2; RMSE = 0.13 μg/L; and MAE = 0.06 μg/L). The successful application of machine learning algorithms emphasizes their potential to elucidate the dynamics of algal biomass in Lake Ranco, located in the southern region of Chile. These results not only contribute to a deeper understanding of the lake ecosystem but also highlight the utility of advanced computational techniques in environmental research and management.

How to cite: Rodríguez-López, L., Bravo Alvarez, L., Duran Llacer, I., Ruíz-Guirola, D., Montejo-Sánchez, S., Martínez-Retureta, R., Bourel, L., Frappart, F., and Urrutia, R.: Leveraging Machine Learning and Remote Sensing for Water Quality Analysis in Lake Ranco, Southern Chile, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-240, https://doi.org/10.5194/egusphere-egu25-240, 2025.

EGU25-2206 | Orals | ESSI3.1

Integrated and Open geohazard monitoring data in Aotearoa New Zealand: developing an interoperable data service for GeoNet’s time series datasets.   

Elisabetta D'Anastasio, Jonathan B. Hanson, Steve Sherburn, Joshua Groom, and Mark Rattenbury

The GeoNet programme at GNS Science Te Pū Ao (GNS) is the primary agency responsible for collecting, managing, and delivering geohazard data in Aotearoa New Zealand, enabling the monitoring of volcanoes, earthquakes, landslides, and tsunamis. The programme oversees a multi-parametric sensor network along with a diverse array of instrumentation and methodologies to provide both raw and analysis-ready data to its end users. Since its inception in 2002, an "open by default" policy has been the guiding principle of this research and monitoring data infrastructure. 

To enhance the interoperability, accessibility, and usability of GeoNet's data, and in alignment with FAIR data principles, we developed an in-house interdisciplinary solution (Tilde) for storing and accessing time-series datasets managed by the programme. Operating successfully for two years, Tilde has improved the interoperability, usability, and FAIR-ness of GeoNet data. In this presentation, we will outline how Tilde has achieved these improvements, discuss challenges and unresolved questions within the geophysical community, and explore potential future directions for leveraging this open data platform to address CARE principles and indigenous data governance in Aotearoa New Zealand. 

How to cite: D'Anastasio, E., Hanson, J. B., Sherburn, S., Groom, J., and Rattenbury, M.: Integrated and Open geohazard monitoring data in Aotearoa New Zealand: developing an interoperable data service for GeoNet’s time series datasets.  , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2206, https://doi.org/10.5194/egusphere-egu25-2206, 2025.

EGU25-2826 | Orals | ESSI3.1

 Datacubes as enablers for land take quantification in LandSupport Regions 

Giuliano Langella, Piero Manna, and Florindo Antonio Mileti

Land take, a significant driver of land degradation, poses challenges for sustainable land management, particularly in regions under high anthropogenic pressure. Addressing these challenges necessitates robust, data-driven approaches to monitor, quantify, and mitigate land take. This contribution explores the integration of datacube technology within the LandSupport Regions platform, leveraging advances from the European LandSupport project and its extension under the Italian GeoSciences-IR project.

Raster datacubes, structured as multidimensional arrays, enable efficient management and analysis of large-scale spatio-temporal datasets, overcoming traditional file-based limitations. The LandSupport Regions platform utilizes a datacube-based Spatial Decision Support System (S-DSS) to enhance the monitoring of land consumption, land cover, and land use at multiple scales—from municipal to national levels. The system integrates heterogeneous datasets, including satellite imagery (e.g., Copernicus), regional land use maps, and environmental indicators (such as high resolution and multi-temporal imperviousness maps), within a common infrastructure, adhering to the FAIR principles.

A key focus is on land take quantification, supported by high-resolution datacubes capable of tracking land-use changes over time. The platform offers decision-makers a suite of tools for generating actionable indicators, assessing compliance with land-use policies, and proposing mitigation strategies aligned with zero net land take objectives. Moreover, the system’s interoperability and open-access characteristics allow integration of user-defined data and models, fostering innovation and scalability.

The platform’s capabilities are demonstrated through use cases in Italy, where local administrations leverage datacube analytics to refine urban and regional planning. These use cases underscore the role of datacubes in delivering accurate, timely insights for sustainable land management. By aligning regional initiatives with European Green Deal objectives, the LandSupport Regions platform – produced under the GeoSciences-IR project – exemplifies the potential of datacube-enabled S-DSSs to advance environmental governance.

How to cite: Langella, G., Manna, P., and Mileti, F. A.:  Datacubes as enablers for land take quantification in LandSupport Regions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2826, https://doi.org/10.5194/egusphere-egu25-2826, 2025.

EGU25-3362 | Orals | ESSI3.1

Mindat: A crowd-sourced and expert-curated open data ecosystem for mineralogy 

Xiaogang Ma, Jiyin Zhang, and Jolyon Ralph

Over the past three years, we have successfully launched an open data service for Mindat, one of the largest databases focused on mineral species and their global distributions. Our achievements include: 1) a comprehensive review of existing data records, covering the list of data subjects, their characteristics, and inherent biases, 2) the establishment of an open data API (application programming interface) alongside Python and R packages to integrate the API into workflow platforms, and 3) fostering community collaboration on data standards and best practices for open data, such as mineral nomenclature, rock classification, and technical frameworks for applying the FAIR (findable, accessible, interoperable, and reusable) principles. Mindat is both crowd-sourced and expert-curated, and for the past decades it has been proven to be an effective approach to engage both data contributors and users. Mindat has been popular amongst geoscience professionals and the public alike. Through our open data initiatives and community engagement, we have also gathered valuable insights to guide future developments of Mindat open data. In this presentation, we will highlight the current open data capabilities, provide an overview of the review of Mindat's data records, and share our vision for leveraging advanced artificial intelligence technologies to expand and enhance Mindat in the future.

How to cite: Ma, X., Zhang, J., and Ralph, J.: Mindat: A crowd-sourced and expert-curated open data ecosystem for mineralogy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3362, https://doi.org/10.5194/egusphere-egu25-3362, 2025.

EGU25-4337 | Orals | ESSI3.1

BEACON - Accelerating access to multidisciplinary data with Relative Optimized Chunking technology 

Robin Kooyman, Peter Thijsse, Dick Schaap, and Tjerk Krijger

Achieving fast access to analysis-ready data from a large number of multidisciplinary data resources is key for contributing to many of the nowadays societal and scientific challenges via Digital Twins of the Oceans or virtual research environments. However, achieving this kind of performance is a major challenge as original data is often organised in millions of (observation) files which makes it hard to achieve fast responses. Next to this, data from different domains are stored in a large variety of data infrastructures, each with their own data-access mechanisms, which causes researchers to spend much time on trying to access relevant data. In a perfect world, users should be able to retrieve analysis-ready data in a uniform way from different data infrastructures following their selection criteria, including for example spatial or temporal boundaries, parameter types, depth ranges and other filters. 

Therefore, as part of several European projects, MARIS has developed a software system called BEACON with a unique indexing and dynamic chunking system that can, on the fly with high performance, extract specific data based on the user’s request from millions of (observational) data files, containing multiple parameters in diverse units. The system returns one single harmonised file as output, regardless of whether the input contains many different data types or dimensions. In January 2025, BEACON 1.0.0 was made publicly available as an open-source software, allowing everyone to set-up their own BEACON node to enhance the access to their data or use existing BEACON nodes from well-known data infrastructures such as Euro-Argo or the World Ocean Database for fast and easy access to harmonized data subsets. More technical details, example applications and general information on BEACON can be found on the website https://beacon.maris.nl/.

The presentation would focus on one of the core features of BEACON called “Relative Optimized Chunking (ROC)”, which is a unique dynamic chunking technology that has been developed specifically to make the data retrieval as fast as possible. This optimized way of chunking reduces the number of chunks BEACON has to search through when a data request has been made. This is done by applying variable sized chunking on multiple levels at the same time such as geo-location, depth and time, which means that data that is relatively close to each other is chunked accordingly. This enhances the speed because it allows BEACON to traverse the millions of datasets using its index with much more precision by not only finding the relevant datasets, but also the exact data blocks containing the relevant data.

The demonstration will involve the use of an existing BEACON node in the field of marine science to access data subsets via its REST API and demonstrate its performance. This will be done in a Jupyter Notebook by querying data via a JSON request to the BEACON system. By going through the Notebook, it will be explained how the BEACON system can be accessed and used by developers including the most recent developments.

How to cite: Kooyman, R., Thijsse, P., Schaap, D., and Krijger, T.: BEACON - Accelerating access to multidisciplinary data with Relative Optimized Chunking technology, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4337, https://doi.org/10.5194/egusphere-egu25-4337, 2025.

EGU25-4843 | Posters on site | ESSI3.1

Aviation Safety Datacubes 

Peter Baumann, Colin Price, Vlad Merticariu, Bang Pham Huu, and Dimitar Misev

Air traffic today is immense, with large numbers of humans and goods transported routinely, but also in search and rescue missions, military contexts, and hobby piloting, etc. Still, aviation today is safer than it ever has been, thanks to advanced technology and procedures which are continuously revisited and, where necessary, improved. Of central importance for planning and conducting flights is the atmospheric condition the aircraft is flying in, represented by various relevant weather parameters. Hence, these are continuously monitored.

In the Cube4EnvSec project, a federated datacube demonstrator has been established which illustrates ad-hoc assessment of atmospheric conditions relevant for aircraft. Data stem from two sources, DWD and WWLLN. 

From German Weather Service (Deutscher Wetterdienst, DWD), WAWFOR (World Aviation Weather Forecast) data are obtained, a digital aviation meteorological dataset based on the ICON6_Nest model in support of air traffic management based on geostationary weather satellites. Components currently used are wind speed, icing parameters, Cumulonimbus tops, temperature, tropopause, turbulence, lightning, precipitation radar, volcanic ash, and dust. Updates are provided every 6 hours, temporal resolution is 1 hour with a forecast window of currently 78 hours. The update batches are harvested from DWD and merged into the respective datacubes, extending it by 6 hours further into the future. The 6 hours not overwritten by the new forecast are retained and create a growing "long tail" of historical weather data, currently about 17,000 timeslices. Some datacubes are 3D x/y/t, most however are 4D x/y/h/t with a spatial resolution of 0.0625° x 0.0625° (approximately 6.5km x 6.5km), altitude between ground and 18,000 feet (FL180).

Lightning data are obtained from the World Wide Lightning Location Network (WWLLN) by the Colin Price research group at Tel Aviv University and aggregated into a 3D x/y/t timeseries of lightning strikes observed. Spatial resolution is 0.1°, temporal resolution is 1 hour.

Altogether, the datacubes have a footprint of currently about 20 TB. APIs offered by the Aviation Safety service include the adopted standards WMS, WMTS, WCS, and WCPS, and additionally the OGC drafts OAPI-Coverages and GeoDataCube. Any client conforming to these APIs can be utilized; in the demonstration the rasdaman dashboard will be used which is configurable for manifold datacube interaction techniques (see Figure at bottom).

The demonstration presented includes the following steps:

  • general overview of the datacubes offered by the service;
  • visualization of the combined forecast/history weather datacubes;
  • information relevant for pilot flight planning: weather hazards overview; severe weather conditions along historic routes;
  • same for ad-hoc chosen flight paths, with 4D corridor cutout;
  • various analytical queries related to flight weather conditions.

Most parts of this demo are publicly accessible under https://cube4envsec.org/aviation-dashboard . Any standard Web browser can access it without any plugin etc. to be installed.

Acknowledgement
Cube4EnvSec has received funding by the NATO Science for Peace and Security (SPS) program.

 

 

 


Fig.: Aviation Safety datacube dashboard

 

How to cite: Baumann, P., Price, C., Merticariu, V., Pham Huu, B., and Misev, D.: Aviation Safety Datacubes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4843, https://doi.org/10.5194/egusphere-egu25-4843, 2025.

EGU25-6020 | Orals | ESSI3.1

AI and Datacubes - a Happy Marriage? 

Dimitar Mishev and Peter Baumann


Datacubes are an accepted cornerstone for Analysis-Ready Data (ARD). One analysis technique of skyrocketing importance today is AI, and this begs the question: how to generalize evaluation of pre-trained models on datacubes?

From a theoretial viewpoint, the connection is immediate: datacubes mathematically resemble tensors, and EO models evaluate tensors. In practice, though, the situation is less straightforward as our experiments with different models have shown. A main issue is the variety and the lack of standardized interfaces of ML models: different input data are processed, data need model-specific preprocessing, and several more. In our research towards offering ML-on-datacubes as a commodity in a federated datacube infrastructure we have collected challenges and methods for presentation.

In our demo, we present AI-Cubes as an enabling concept uniting AI and datacubes. The demos will approach the theme from two sides:

- AI support for datacube query writing: We have trained a chatbot to explain and assist with datacube queries in the OGC/ISO/INSPIRE WCPS standard. This can act as a productiity-enhancing tool for both expert and non-expert users. We demonstrate live how specific questions get answered, such as phrasing NDVI on Sentinel-2 data.

- AI model evaluation on datacubes: particularly attractive is that datacubes allow simple navigation to any area, any time, and even from federated services. This we demonstrate live.

We also highlight challenges coming with this simple data access: models do not convey the same performance anywhere, anytime. This has led to new research on "model fencing", ie: attempting to restrict model application to situations where they exhibit sufficient accuracy. We present first ideas of this research.

Altogether, we cast light on the combination of datacubes and AI from a service and infrastructure perspective. 

How to cite: Mishev, D. and Baumann, P.: AI and Datacubes - a Happy Marriage?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6020, https://doi.org/10.5194/egusphere-egu25-6020, 2025.

EGU25-7038 | Posters on site | ESSI3.1

Establishing Institutional Workflows to Engage Stakeholder Groups in PID Metadata Maintenance 

Emanuel Soeding, Dorothee Kottmeier, Andrea Poersch, Stanislav Malinovschii, and Sören Lorenz

At the Helmholtz Association, we strive to establish a well-structured, harmonized data space that seamlessly connects information across distributed data infrastructures. Achieving this goal requires the standardization of dataset descriptions through consistent metadata practices, such as leveraging persistent identifier (PID) metadata, to ensure interoperability and machine actionability.

While developing concepts to harmonize PID metadata is a crucial first step in creating a unified data space, it is not sufficient on its own. The practical application of PIDs to facilitate the compilation of rich, relevant metadata for datasets necessitates knowledge, training, support, and cooperation among diverse stakeholder groups, each responsible for different aspects of the information lifecycle.

For example, ORCID is a PID system designed to identify individuals contributing to research. Traditionally, this has primarily applied to scientists publishing journal articles. However, in the context of research data, other stakeholders also play vital roles. These include technicians operating instrumentation, data management personnel curating research data and repositories, and administrative staff maintaining institutional data relevant to research. Currently, these stakeholders are often unaware of their potential roles in data management, and the information they collect is typically not harmonized. To address this, workflows must be implemented to manage, structure, and connect the information they produce to research data where appropriate. In the case of ORCID, these workflows should begin at the earliest stages of the research process, such as during employee onboarding.

PIDINST, a PID system introduced by an RDA working group, provides a simple metadata schema to collect essential information about instruments and registers them with unique IDs. These IDs are invaluable for identifying measurements conducted with the same or similar devices. Therefore, we strongly recommend the adoption of PIDInst within the Helmholtz Association. For PIDINST, successful implementation would involve integrating the workflow into existing processes, starting with the acquisition of an instrument or sensor at the research center. Relevant information would then be passed to technicians responsible for maintaining up-to-date records. For researchers, PIDINST provides reliable identification of devices used in scientific processes.

In this presentation, we highlight critical positions within the centers where minor adjustments to established workflows can significantly support the registration of specific PIDs and the engagement of stakeholder groups. We also explore strategies for implementing these changes across the Helmholtz Association. Furthermore, we assign clear responsibilities for metadata maintenance to appropriate stakeholders. The conclusions drawn from this process aim to redefine roles and responsibilities within our organization, fostering a more integrated and effective approach to data management.

How to cite: Soeding, E., Kottmeier, D., Poersch, A., Malinovschii, S., and Lorenz, S.: Establishing Institutional Workflows to Engage Stakeholder Groups in PID Metadata Maintenance, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7038, https://doi.org/10.5194/egusphere-egu25-7038, 2025.

The World Data System (WDS), a member of the International Science Council, serves a membership of over 150 trusted data repositories and related organizations. It builds on the data sharing legacy of World Data Centers that were initiated seven decades ago. Governed by a Scientific Committee, the WDS consists of an International Program Office (WDS-IPO) based in Oak Ridge, Tennessee, USA, and an International Technology Office (WDS-ITO) based in Victoria, BC, Canada. The WDS mission is to enhance the capabilities, impact, and sustainability of our member data repositories and data services. In this presentation, we outline the 2025 to 2027 Action Plan objectives, highlighting activities and collaborations that are underway or planned to progress open science, integrated data infrastructures and FAIR/CARE/TRUST Principles. 

How to cite: Jenkyns, R.: Advancing Open Science through Trusted Data Repository Intersections at the World Data System, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7551, https://doi.org/10.5194/egusphere-egu25-7551, 2025.

EGU25-7959 | Orals | ESSI3.1

Breaking down data sharing barriers and uplifting FAIR for climate data at scale 

Clare Richards, Kelsey Druken, Romain Beucher, and Felicity Chun

Developing climate models often requires the ability to access and share extremely large datasets (spanning tens to hundreds of terabytes) that are discoverable and optimised for high-performance computing (HPC) applications. This is a major challenge, as researchers frequently lack the storage resources and specialised support needed to ensure efficient data management and sharing practices across the full data life-cycle. The challenges of sharing data are evident even when dealing with curated datasets that are prepared for broad access, citation, and reuse. However, these challenges are amplified during the rapid and iterative stages of model development and prototyping. At this point, multiple versions of datasets must be shared and evaluated by a wide range of experts before the data is finalised and curated for public use. This iterative process requires robust infrastructure and coordination to avoid bottlenecks that can hinder progress.

To help overcome these barriers, Australia’s Climate Simulator (ACCESS-NRI) provides a dedicated merit allocation scheme for compute and storage resources. This includes 3PB of storage for datasets that are for use by community members to undertake scientific research, support model development and/or will be shared for reuse. Experience has shown, that if the usage of these storage resources is not managed then the data can quickly go from being an asset to a liability.  Therefore, to maximise the value of both the data and investment in storage, ACCESS-NRI has developed an approach for sharing datasets that is designed to support science and innovation while enhancing the current practices for making data more accessible and usable in accordance with the FAIR and CARE principles.

We will present the motivating use cases and show how this approach supports the model development cycle while making data and the science it underpins more transparent, open and accessible. This approach encourages data generators to transition their datasets from unmanaged, undocumented spaces into managed environments where curation and oversight are aligned with the data’s intended purpose and use. It acknowledges that supporting FAIR principles does not always require full curation to the standards of a long-term publication. Instead, it focuses on reducing barriers to data sharing by promoting active data management practices. These practices enhance discoverability, trust, and reliability, ensuring that shared data is fit for purpose without imposing unnecessary burdens.

ACCESS-NRI is a national research infrastructure (NRI) established to support the Australian Community Climate and Earth System Simulator, or ACCESS. The ACCESS suite of software and data outputs are essential tools used to simulate past and future climate, weather and Earth systems and to support research and decision making within Australia.

ACCESS-NRI's mission is to build an open collaborative infrastructure that will accelerate research in Earth system, climate and weather modelling as well as enable new research not currently possible. The facility brings together skills in software development, high-performance computing, data management and analysis to enhance the ACCESS modelling framework, making it easier to use and lowering the barrier for scientific innovation.

How to cite: Richards, C., Druken, K., Beucher, R., and Chun, F.: Breaking down data sharing barriers and uplifting FAIR for climate data at scale, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7959, https://doi.org/10.5194/egusphere-egu25-7959, 2025.

EGU25-9104 | Orals | ESSI3.1

Using Data Cubes to Investigate Links Between Lightning and Civil Aviation 

Colin Price, Aviv Shay, and Peter Baumann

Lightning is a hazard for many sectors and industries, including the power utility sector, wind turbines, forest management, and civil aviation.  Commercial aircraft are struck by lightning approximately once every year, but most airlines try to avoid thunderstorms if possible by rerouting around these turbulent and electrified storms.  However, such diversions can delay flights, add costs to fuel demands, while increasing greenhouse gas emissions for the aircraft company.  In this study using data cubes we have combined lightning data from the World Wide Lightning Location Network (WWLLN) together with civil aviation flight data from FlightRadar24 to better understand the risks of lightning to civil aviation.  Combining historic lightning and aviation data we can address questions about risks to aircraft from thunderstorms, the frequency of close encounters with thunderstorms, and the frequency of rerouted flights due to thunderstorm activities.  The emerging concept of Analysis-Ready Data (ARD) attempts to find concepts and methods towards services operating on homogenized data. For spatio-temporal data, datacubes are an accepted cornerstone for ARD providing Big Geo Data easier for users and applications, ready for analysis, visualization, fusion, etc. As part of the Cube4EnvSec NATO Science for Peace and Security (SPS) project we will present live demos of our data cube tools and services related to lightning risks for civil aviation over Europe.  Derived analytics from the datacube will also be presented.

How to cite: Price, C., Shay, A., and Baumann, P.: Using Data Cubes to Investigate Links Between Lightning and Civil Aviation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9104, https://doi.org/10.5194/egusphere-egu25-9104, 2025.

EGU25-10578 | Orals | ESSI3.1

DynAWI Extreme Weather Toolbox: an online platform for agricultural risk assessment and decision support 

Arno de Kock, Timm Waldau, Pedro Batista, Peter Baumann, Thorsten Behrens, Peter Fiener, Jens Foeller, Markus Moeller, Ingrid Noehles, Karsten Schmidt, and Burkhard Golla

The DynAWI Extreme Weather Toolbox represents an innovative approach to addressing climate-related challenges in agriculture. This publicly accessible web application offers three primary functions: a historical agricultural weather indicator atlas, a dynamic configurator for calculating user-specified weather indexes, and a forecast model for predicting reduced yields or complete crop failure due to weather extremes. The web application can perform real-time analyses based on multi-dimensional spatio-temporal data.

The technical implementation is based on a client-server architecture, utilizing a scalable geodata infrastructure and an array database management system rasdaman, enabling efficient processing of multidimensional geodata. The system allows real-time analysis of extreme weather events, such as droughts, heatwaves, and heavy rainfall, dating back to 1995. The toolbox aims to provide stakeholders—from farmers to policymakers—with a comprehensive platform for weather-related risk assessment and decision support in agriculture.

In a live demonstration, we will showcase the platform's key features, emphasizing its interactive capabilities and extensive parameter customization options.

How to cite: de Kock, A., Waldau, T., Batista, P., Baumann, P., Behrens, T., Fiener, P., Foeller, J., Moeller, M., Noehles, I., Schmidt, K., and Golla, B.: DynAWI Extreme Weather Toolbox: an online platform for agricultural risk assessment and decision support, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10578, https://doi.org/10.5194/egusphere-egu25-10578, 2025.

EGU25-10583 | Orals | ESSI3.1

EOEPCA+: a method for an open-sourced EO Exploitation Platform Common Architecture 

Richard Conway, James Hinton, Chandra Taposeea, Claudio Iacopino, Salvatore Pinto, and Simon Hunter

The ‘Exploitation Platform’ concept derives from the need to access and process an ever-growing volume of data. Many web-based platforms have emerged - offering access to a wealth of satellite Earth Observation (EO) data, increasingly collocated with cloud computing resources and applications for exploiting the data. Rather than downloads, the exploitation platform offers a cloud environment with EO data access and associated compute and tools facilitating the analysis and processing of large data volumes. Users benefit from the scalability & performance of the cloud infrastructure, the added-value services offered by the platform – and avoid the need to maintain their own hardware. Data hosted in the cloud infrastructure reaches a wider audience and Infrastructure Providers gain an increased cloud user base.

Users are beginning to appreciate the advantages of exploitation platforms. However, the market now offers a plethora of platforms with various added value services and data access capabilities. This ever-increasing offer is intimidating and confusing for most users, often facing challenges such as inconsistent interfaces, proprietary software and limited interoperability. To fully exploit the potential of these complementary platform resources, interoperation amongst the platforms is needed, such that users of one platform may consume the services of another directly platform-to-platform.

EOEPCA (EO Exploitation Platform Common Architecture) is a European Space Agency (ESA) funded project with the goal to define and agree a re-usable exploitation platform architecture using standard interfaces to encourage interoperation and federation between operational exploitation platforms - facilitating easier access and more efficient exploitation of the rapidly growing body of EO and other data. Interoperability through open standards is a key guiding force for the Common Architecture. EOEPCA adheres to standards from organisations such as Open Geospatial Consortium (OGC) and follows best practices in data management, including implementation of OGC Web Services and emerging OGC API specifications for features, coverages and processes. Platform developers are more likely to invest their efforts in standard implementations that have wide usage; off-the-shelf clients and software are more likely to be found for standards-based solutions.

The EOEPCA system architecture is designed to meet defined use cases for various user levels(expert application developers to data analysts and end users). The architecture is defined as a set of Building Blocks (BBs), exposing well-defined open-standard interfaces. These include Identity and Access Management, Resource Discovery, Data Access, Processing Workflows, Data Cube Access, Machine Learning Operations, and more. Each of these BBs are containerized for Kubernetes deployment, providing an infrastructure-agnostic deployment target.

The exploitation platform is conceived as a ‘virtual work environment’,  withusers accessing data, developing algorithms, conducting analysis and sharing value-adding outcomes. The EOEPCA architecture facilitates this through a Workspace BB, providing collaboration environments for groups of users, including dedicated storage and services for analysis, processing and publishing of added-value data and applications. This is supported by an Application Hub BB, providing interactive web-tooling for analysis, algorithm development, data exploitation and providing a web dashboard capability, whereadded-value outcomes are showcased.

Our presentation will highlight the generalised architecture, standards, best practice and open source software components available.

How to cite: Conway, R., Hinton, J., Taposeea, C., Iacopino, C., Pinto, S., and Hunter, S.: EOEPCA+: a method for an open-sourced EO Exploitation Platform Common Architecture, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10583, https://doi.org/10.5194/egusphere-egu25-10583, 2025.

EGU25-10638 | Orals | ESSI3.1

Climate Science Meets Data Spaces: FAIR Digital Objects as a Gateway to Interdisciplinary Science 

Ivonne Anders, Beate Krüss, Marco Kulüke, Karsten Peters-von Gehlen, Hannes Thiemann, and Heinrich Widmann

In recent years, the concept of data spaces has gained prominence, particularly in industry, as a framework for organizing and sharing data across business ecosystems and institutional and disciplinary boundaries. While the term itself is not yet widely adopted in the scientific community , it can be directly applied to research. Data spaces provide a  structured environment for integrating data sets from diversedisciplines, methods or fieldsand making themaccessible for collaboration and analysis. Climate and climate impact research, which relies on data from different fields such as meteorology, hydrology or socio-economics, is in a unique position to benefit from the application from this approach.

In line with the principles of open science, researchers are increasingly adopting frameworks that promote transparency, accessibility and reproducibility. FAIR Digital Objects (FDOs) offer effective means of achieving these goals while also enabling interactions between different data spaces. As standardized, interoperable, and machine-readable entities, FDOs link data, metadata and software, simplifying integration and promoting reuse across disciplines.

Using an example from climate research, we demonstrate how climate model data from an institutional data space, observational data from field campaigns, and satellite data (e.g., from the Destination Earth Data Lake) can be combined. By employing STAC (Spatio Temporal Asset Catalog) catalogs defined as FAIR Digital Objects facilitating the European Open Science Cloud (EOSC) Data Type Registry, we address a specific interdisciplinary research question. This approach not only illustrates the practical application of FDOs but also highlights how they can provide a robust framework for tackling larger and more complex scientific challenges by streamlining workflows and enabling collaboration across disciplinary and institutional boundaries.

How to cite: Anders, I., Krüss, B., Kulüke, M., Peters-von Gehlen, K., Thiemann, H., and Widmann, H.: Climate Science Meets Data Spaces: FAIR Digital Objects as a Gateway to Interdisciplinary Science, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10638, https://doi.org/10.5194/egusphere-egu25-10638, 2025.

EGU25-15095 | Orals | ESSI3.1

Advancing Open, FAIR, and Responsible Science through the International Generic Sample Number 

Rorie Edmunds, Jens Klump, Kirsten Elger, Lesley Wyborn, Kerstin Lehnert, Lindsay Powers, and Fabian Kohlmann

Research to address global environmental and societal challenges increasingly depends on the availability of large-scale, multidisciplinary datasets, making the need for robust systems that ensure data discoverability, accessibility, and interoperability evermore critical. However, having the data is not enough, one also needs to know about—and understand the connections among—related outputs and entities that support the veracity and reproducibility of the research.

The International Generic Sample Number (IGSN) is a persistent identifier (PID) for material samples arising from any research discipline. Originally developed in the Earth Sciences, the IGSN provides a vital component in solving the abovementioned challenges, enabling seamless integration of sample data across diverse platforms, disciplines, and organizational and geographic boundaries. By uniquely and permanently linking samples to their descriptions (provided as structured metadata), analytical results, and associated publications, IGSNs facilitate transparency, traceability, and reusability of material samples in line with the FAIR and CARE Principles. This is underpinned by the proven interoperability of the IGSN with the scientific communication infrastructure, which also enables citations of samples in the literature to be automatically captured.

This presentation will showcase the collaborative efforts of the IGSN Organization (IGSN e.V.) and DataCite to establish a resilient, cross-disciplinary, globally harmonized PID system for material samples. Use cases will illustrate how IGSNs enhance research workflows, enabling researchers to be more effective and attributed. We will also discuss governance, technical standards, and best practices that promote trust in the IGSN-DataCite partnership and scalability of sample PID adoption, aligning with UNESCO’s Open Science recommendations.

How to cite: Edmunds, R., Klump, J., Elger, K., Wyborn, L., Lehnert, K., Powers, L., and Kohlmann, F.: Advancing Open, FAIR, and Responsible Science through the International Generic Sample Number, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15095, https://doi.org/10.5194/egusphere-egu25-15095, 2025.

EGU25-16668 | Posters on site | ESSI3.1

The Visual Drill Core Library: A Tool for Improving Access to Samples from the Natural Science Institute of Iceland 

María Helga Guðmundsdóttir, Kjartan Birgisson, Hrafnkell Hannesson, Kristján Jónasson, Anette Th. Meier, Birgir Vilhelm Óskarsson, and Björn Darri Sigurðsson

The Drill Core Library (DCL) of the Natural Science Institute of Iceland is Iceland’s national repository for drill cores and cuttings. As such, the DCL is responsible for preserving these geological samples and making them available to the scientific community. The library comprises an estimated 100 km of core and a 470 km equivalent of cuttings from over 4,000 boreholes, as well as a growing database of analytical results. The collection spans Iceland’s range of diverse geological environments and houses core from significant research projects including the SUSTAIN drilling project in Surtsey, sponsored in part by the International Continental Scientific Drilling Program, and the Iceland Research Drilling Project. The DCL’s drill cores and cuttings are available for study and sampling for research purposes, and DCL staff are available for consultation and assistance in identifying and collecting suitable samples. The DCL’s on-site facilities are maintained in collaboration with the University of Iceland’s Research Centre in Breiðdalsvík, East Iceland.

An emphasis has been placed on developing digital infrastructure to improve access to the collections for the scientific community. To facilitate sample identification, an online map-based interface and WFS service have been created where the collection can be examined and contextualized with geological data. The database of the DCL has also been partly integrated into the European Plate Observing System (EPOS), a collaborative initiative enabling FAIR (Findable, Accessible, Interoperable, and Reusable) and open access to geoscientific data from across Europe.

The latest advance in digital access is the ongoing population of the DCL database with core photographs. These are linked directly to the WFS and map viewer, forming a “visual library” that enables direct examination of the library collections, thereby facilitating identification of sampling targets by researchers around the world. At present, 16% of the drill core collection has already been photographed, with 50% set as a target for the end of 2025. Further development of the interface will be carried out in consultation with users of the DCL collections, and cores of interest to researchers are prioritized for photography.

How to cite: Guðmundsdóttir, M. H., Birgisson, K., Hannesson, H., Jónasson, K., Meier, A. Th., Óskarsson, B. V., and Sigurðsson, B. D.: The Visual Drill Core Library: A Tool for Improving Access to Samples from the Natural Science Institute of Iceland, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16668, https://doi.org/10.5194/egusphere-egu25-16668, 2025.

EGU25-16708 | ECS | Orals | ESSI3.1

Scalable and Interoperable Datacube Framework for Advanced Geospatial Data Analysis 

Chen-Yu Hao, Jo-Yu Chang, I-Liang Shih, and Ya-Chu Change

This study introduces a scalable and integrated datacube framework for efficient geospatial data processing and analysis. Leveraging the advanced cloud infrastructure of the National Center for High-Performance Computing (NCHC), the framework combines the openEO API and OGC services to address challenges in managing multidimensional datasets. By ensuring interoperability, security, and high-performance computing, the framework provides a reliable solution for researchers and practitioners to tackle complex geospatial challenges.

Framework Architecture

The framework architecture integrates advanced tools and services, focusing primarily on the openEO API and OGC standard services (e.g., Web Coverage Service and Web Coverage Processing Service). The openEO API provides a unified interface supporting multiple programming languages, allowing users to design and execute customized workflows and enabling batch processing.

openEO integration
The openEO API plays a central role in the framework, performing the following functions:

  • Unified Data Access and Processing Interface: openEO offers a standardized access and processing layer for Earth observation data, abstracting underlying complexities and enabling users to uniformly access multidimensional data from various sources, such as satellite imagery and terrain datasets.
  • Process Graphs and User-Defined Processes: openEO supports User-Defined Processes and Process Graphs, enabling users to create tailored data processing pipelines based on specific analytical requirements. This is particularly valuable for advanced analyses like temporal change detection or spatial statistics.
  • Seamless Integration with OGC Services: openEO works seamlessly with OGC services (e.g., WCS and WCPS) in the framework, enhancing its ability to handle multi-source data. While openEO provides high-level data access and analytical capabilities, OGC services ensure interoperability and standardization at the data layer.

API Proxy Architecture Design

The API proxy is a critical component of the framework, bridging the openEO API and the backend infrastructure to ensure efficient, secure, and stable interactions between users and the system. Its main functions include authentication, authorization management, traffic control, and caching. With the API proxy, openEO can provide a simplified user experience while ensuring optimal utilization of backend data and resources.

Application Scenarios

1. Terrain Analysis
By transforming digital terrain models (DTMs) into multidimensional structures, the framework significantly improves the processing speed and accuracy of large-scale datasets. openEO’s role includes providing a unified interface for data access, enabling users to quickly retrieve and process data for custom slope calculations, visibility analyses, and more. Simultaneously, API proxy security layers ensure strict management of data access and usage.

2. Temporal Analysis Using Landsat Imagery
Temporal analysis of Landsat imagery involves handling large volumes of time-series data. Here, openEO acts as the analytical hub, allowing users to submit analysis requests (e.g., calculating the Normalized Difference Water Index (NDWI)) via the API. The framework then automatically invokes OGC services for data processing and result generation.

Conclusion

The proposed datacube framework successfully integrates openEO API and OGC services, offering a scalable, interoperable, and high-performance solution. As a unified data access and analytical interface, openEO provides flexible and robust tools that significantly simplify complex data processing workflows. By lowering technical barriers and enhancing analytical accessibility, the framework delivers unprecedented convenience for geospatial data analysis, making it a key tool in research and decision-making processes.

How to cite: Hao, C.-Y., Chang, J.-Y., Shih, I.-L., and Change, Y.-C.: Scalable and Interoperable Datacube Framework for Advanced Geospatial Data Analysis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16708, https://doi.org/10.5194/egusphere-egu25-16708, 2025.

EGU25-18594 | Orals | ESSI3.1

FAIRification of sensor-based time-series data – a demonstration of the Helmholtz DataHub digital ecosystem  

Benjamin Louisot, Roland Koppe, Robin Heß, Ulrich Loup, Jürgen Sorg, Marc Adolf, Claas Faber, Andreas Lehmann, Nils Brickmann, Marc Hanisch, David Schäfer, Linda Baldewein, Ulrike Kleeberg, Marie Ryan, Sabine Barthlott, Christof Lorenz, Florian Obersteiner, and Hylke van der Schaaf

In environmental sciences, observational data remains indispensable for monitoring and understanding of natural processes, validating earth system models and remote sensing products, and training of data driven methods. However, unified standards and interfaces for ensuring that such data is consistently available, usable, and compliant with FAIR and Open Science principles are still lacking.

The so-called DataHub initiative of the Helmholtz Research Field Earth & Environment, involving seven large environmental research Centers across Germany, addresses this gap by collaboratively developing a cohesive and unified research data space, including consistent data formats, metadata standards, tools, interfaces and services.

Since the beginning of the DataHub, we have been particularly focusing on unifying time-series data from environmental sensor systems, which are operated across all participating Centers. In this context, we have developed a digital ecosystem, that enhances and links existing and established research data infrastructures with well-defined interfaces and metadata standards. This ecosystem now covers the full processing chain from the integration of new sensor systems and their metadata over automatic and manual quality checks and flagging schemes to the visualization via dashboards and data portals or the usage in data analysis frameworks. In particular, our framework consists of multiple independent tools and services like the Sensor Management System (Brinckmann et al., 2024) as dedicated system for managing sensor metadata, the System for Automated Quality Control (SaQC, Schäfer et al. 2024) as common framework for QA/QC, a tailored metadata profile which adapts the SensorThings API (STA) from the Open Geospatial Consortium to common requirements from environmental sciences (Lorenz et al. 2024), the Earth Data Portal (https://earth-data.de) as overarching data portal and visualization suite as well as tools and services that link all these different building blocks.

While the first concepts of this ecosystem were based on temporary tools and interfaces, we have now reached a level of maturity, that allows us to confidently scale our solutions to new communities and user groups. In this presentation, we will hence give a brief overview of our ecosystem as well as the integrated tools and services. The main focus will be on a hands-on demonstration of the full workflow from deploying a new sensor system, the integration into the contributing services, the (meta)data provision via STA as well as the integration in different downstream systems like the Earth Data Portal for data visualization.

By this, we want to promote the potential of a decentralized research data infrastructure, that has been developed and adopted across multiple research Centers and reach out for new communities and user groups for ultimately creating a FAIR and inter-institutional open data space for our environmental sciences.

How to cite: Louisot, B., Koppe, R., Heß, R., Loup, U., Sorg, J., Adolf, M., Faber, C., Lehmann, A., Brickmann, N., Hanisch, M., Schäfer, D., Baldewein, L., Kleeberg, U., Ryan, M., Barthlott, S., Lorenz, C., Obersteiner, F., and van der Schaaf, H.: FAIRification of sensor-based time-series data – a demonstration of the Helmholtz DataHub digital ecosystem , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18594, https://doi.org/10.5194/egusphere-egu25-18594, 2025.

EGU25-18601 | ECS | Orals | ESSI3.1

OceanUCA: Technological innovation for the management and communication of coastal data in Andalusia through numerical modelling and open source technology. 

Jerimar Vasquez Rojas, Juan Carbone, Alfredo Izquierdo González, Javier Benavente González, Jesús Gómez Enri, Tomás Fernández -Montblanc, Flavio Martins, William Cabos Narvaez, Carlos Yagüe, Carlos Román-Cascón, Oscar Álvarez, Caio Fonteles, Bruno Marques, and Francisco Campuzano

The main objective of the OceanUCA project is the modernization of the technological infrastructure of the University of Cadiz in relation to atmospheric and hydrodynamic numerical modeling specifically configured to simulate physical processes on the coast of Andalusia (Spain).
The initiative focuses on the improvement of modeling systems (oceanographic and atmospheric) and the modernization of servers, mainly THREDDS and ERDDAP. THREDDS facilitates connectivity between scientific data providers and end users, while ERDDAP simplifies the sharing and visualization of time series data through common formats, graphics and maps. The project aims to optimize access, organization and storage of data, create a complete data bank and standardize protocols.
For the storage of data from numerical models, a file server is acquired that allows the custody of large volumes of information related to simulated physical processes, especially focused on the Andalusian coasts. In the future, this server will also facilitate the storage of data from other sources for further calculation, processing and sampling. This acquisition contributes to centralizing the files, currently distributed across different storage sources, and to improving communication across the THREDDS/ERDDAP servers.
The project includes a web application that presents the models in a user-friendly and interpretable format, especially for the scientific community, through the visualization of images.
The technological infrastructure will allow significant advances by facilitating the download of numerical data and taking advantage of graphical processing and high-performance computing to process large data sets. This approach improves the scalability and resolution of forecasts, making them more accessible to the public. By adopting an open-source framework, the project promotes collaboration and knowledge sharing at national and international scales, empowering both the scientific community and the public to use coastal and atmospheric data for informed decision-making and sustainable resource management.

How to cite: Vasquez Rojas, J., Carbone, J., Izquierdo González, A., Benavente González, J., Gómez Enri, J., Fernández -Montblanc, T., Martins, F., Cabos Narvaez, W., Yagüe, C., Román-Cascón, C., Álvarez, O., Fonteles, C., Marques, B., and Campuzano, F.: OceanUCA: Technological innovation for the management and communication of coastal data in Andalusia through numerical modelling and open source technology., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18601, https://doi.org/10.5194/egusphere-egu25-18601, 2025.

EGU25-19278 | Orals | ESSI3.1

One platform will not solve everything: How FID GEO strengthens Germany’s Open Science Landscape for the geosciences. 

Melanie Lorenz, Kirsten Elger, Inke Achterberg, and Malte Semmler

The Specialized Information Service for Geosciences (FID GEO) is a German Research Foundation (DFG)-funded initiative that has been serving the geoscience community in Germany for almost a decade. FID GEO provides essential publication services through its partner domain repositories GFZ Data Services (for research data and software) and GEO-LEOe-docs (for text publications). Beyond these repositories, FID GEO actively supports the digital transformation and supports researchers in adopting Open Science practices mainly through workshops, publications, conference contributions and active participation in topic-specific meetings. 

Collaboration is a cornerstone of FID GEO’s work. It engages closely with geoscientific societies, national infrastructures and initiatives such as the German National Research Data Infrastructure (NFDI), while also contributing to policy-making processes such as the planned German Research Data Act. Recognizing the inherently global nature of geosciences, FID GEO further aligns its activities with international developments, striving to synchronize national progress with global standards and best practices for data management and distribution. FID GEO acts as an interface between scientists, libraries, repositories and the world of digital data management and thus support the transformation of the publication culture in the geosciences at national and international level.

For many years, FID GEO has received feedback from researchers expressing a strong desire for a ‘single source’ platform to manage and share their increasingly large datasets, publications, and projects. At the same time, researchers often feel overwhelmed by the complexity and number of existing infrastructures. However, not only does a one-size-fits-all solution appear technically out of reach, it also faces issues in scalability and sustainable maintenance. A viable way forward is the widespread implementation of machine-readable (meta)data standards that also enable the connection between distributed data systems. Additional metadata properties enable persistent digital links between different research outputs and the unique identification of authors and institutions through persistent identifiers. Another significant challenge within the research landscape is the often competing nature of infrastructures, driven by limited funding opportunities and overlapping goals. Through its extensive network and active collaborations, FID GEO addresses these challenges by guiding researchers through this complex landscape and demonstrates practical ways to make their scientific outputs visible, reusable, and aligned with the FAIR and Open Science principles.

This presentation will share best practices, lessons learned, and future directions for fostering a collaborative and open research environment. FID GEO envisions a geoscience community empowered by shared data and cooperative infrastructures, better equipped to address pressing global challenges.

How to cite: Lorenz, M., Elger, K., Achterberg, I., and Semmler, M.: One platform will not solve everything: How FID GEO strengthens Germany’s Open Science Landscape for the geosciences., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19278, https://doi.org/10.5194/egusphere-egu25-19278, 2025.

EGU25-19453 | Orals | ESSI3.1

ESGF Next Generation and preparations for CMIP7 

Rhys Evans, David Poulter, Philip Kershaw, Ian Foster, Rachana Ananthakrishnan, Forrest Hoffman, Aparna Radhakrishnan, Stephan Kinderman, Sasha Ames, and Daniel Westwood

The Earth System Grid Federation (ESGF) is the international partnership responsible for the distribution, cataloging and archiving of both the Coupled Model Intercomparison Project (CMIP) and the Coordinated Regional Climate Downscaling Experiment (CORDEX). In operation since 2009, it was the first decentralised climate data repository of its kind, storing and serving many petabytes of data across tens of global and region data centre partners.

Over the last five years, the system has been fully rearchitected, introducing a cloud-ready deployment architecture and a new system for distributed search, fundamental to ESGF’s federated model for data access. This has involved innovations, translating successful experience with the STAC (Spatio-Temporal Asset Catalogue) specification from the EO world and developing a profile for its use with global climate projections data. Providing a STAC interface to ESGF archives has allowed us to explore alternate access methods for cloud-accessible analysis-ready data ready formats through the use of tools such as Kerchunk, a lightweight non-conversion approach for referencing existing data, which works with open-source python packages like fsspec and Xarray. Use of STAC also provides the potential for greater integration between EO and climate modelling domains essential for the validation of model outputs.

ESGF has traditionally used a distributed model for search services which though powerful has led to challenges around consistency of search content. Over the last twelve months, in preparation for CMIP7, a further fundamental innovation has been made in the architecture to address these issues. The new system adopts a centralised model, with two search nodes, one in the US and one in Europe each hosted on public cloud. These two nodes are synchronised together using a new event-driven architecture. This approach, driven by a shared messaging framework between the nodes, ensures eventual-consistency across the nodes, to reduce or eliminate errors caused by individual node down time and simplify processes such as the replication and retraction of data from the archives distributed at sites across the federation.

The move to a message based, event driven architecture has been integrated with STAC records and services. In ESGF-NG data is shared between nodes as messages in the form of STAC Item records, ensuring a consistent, publicly documented archive distributed across many nodes. The ESGF team have contributed several changes to the STAC project to facilitate this change. Looking forward, we see potential in this new event driven architecture for search systems as a means to integrate across federations - in the European context this could include the ESA Climate Change Initiative open data portal, work with the Copernicus Climate Data Store and DestinE.

How to cite: Evans, R., Poulter, D., Kershaw, P., Foster, I., Ananthakrishnan, R., Hoffman, F., Radhakrishnan, A., Kinderman, S., Ames, S., and Westwood, D.: ESGF Next Generation and preparations for CMIP7, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19453, https://doi.org/10.5194/egusphere-egu25-19453, 2025.

EGU25-20533 | Orals | ESSI3.1

A Grass-roots Standard for Time Series Data in any Domain: HAPI 

Jon Vandegriff, Robert Weigel, Jeremy Faden, and Alexander Antunes

We describe a simple interface for accessing time series numeric data: the Heliophysics Application Programmer's Interface (HAPI). Although it started in NASA's Heliophysics domain, no Heliophysics idioms are present in the standard, and HAPI can be used to serve any tabular, numeric data that is indexed by time.  HAPI was the result of a community push to standardize similar access methods at multiple data centers, and it is now in use at 12 data centers around the world, with over 12,000 datasets available in a standard way. HAPI offers a more conceptual view of the data, independent of the storage arrangements at a server. It also is not intended to replace an existing server's API, but to sit alongside that API.  The project is mature, with a reference server available, as well as clients in multiple programming languages.  We will present an overview of the API and compliance with FAIR principles. We also will describe some of the visualization and analysis tools being developed now that standardized access is becoming a reality. We invite discussion with other time series data providers in other domains.

How to cite: Vandegriff, J., Weigel, R., Faden, J., and Antunes, A.: A Grass-roots Standard for Time Series Data in any Domain: HAPI, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20533, https://doi.org/10.5194/egusphere-egu25-20533, 2025.

EGU25-20550 | Orals | ESSI3.1

Are Publicly Funded Data-Infrastructures Reliable? 

Hans Pfeiffenberger and David Carlson

As founders and former chief editors of Earth System Science Data (ESSD), the authors are concerned about the reproducibility and availability of important scientific sources and findings, and about timely access to scientific data and data-related services. We are discussing (1) incidents with the availability of DOIed datasets and their metadata and (2) a recent outage of an important data infrastructure.

Both observations are considered sufficiently serious that the authors wonder why the underlying facts and realities are not discussed widely in this community.

1) The most cited dataset published through ESSD is the series of yearly reports on the Global Carbon Budget, e.g. the latest, https://doi.org/10.5194/essd-2024-519. These articles are cited in scientific publications by the hundreds of times and routinely inform the United Nations climate change conferences (COPs). The first datasets of the series were held and provided DOIs by the Carbon Dioxide Information Analysis Center (CDIAC), which was hosted by the Oak Ridge National Laboratory. When CDIAC was shut down in 2017, the datasets were transferred to a repository at another US National Lab, loosing most of the metadata in the process, most notably authorship. Thankfully, hosting of post-2017 additions to the dataset series has been taken over by the Integrated Carbon Observing System (ICOS) and DOIs to all elements of the series still resolve (albeit, in a sloppy manner for pre-2018 data). One could argue that the most reliable holder of metainformation about this – not just scientifically – important data are not the repositories but ESSD, operated by a commercial publisher, Copernicus. 

2) When tropical storm Helene hit North Carolina, in September 2024, power and internet connectivity went out from the Asheville headquarter site of NOAA’s NCEI, an aggregator, archive and service provider for environmental data. Although NCEI is hosted at four geographically dispersed sites, NCEI data ingest and services came to a halt for several weeks. It appears that most data from the period during and after Helene have been collected retroactively, and services are fully available again. While NOAA’s real-time weather services, important to deal with the emergency, seem to have been available during Helene, one is tempted to ask if they could become interrupted under similar circumstances.

Both these and some other observations – which will be discussed at EGU2025 - create the uncomfortable impression that the huge efforts of this community wrt. the FAIRness of data and in the creation of a multitude of publicly funded infrastructure elements do not achieve to meet today’s needs, and possibly may not meet them tomorrow. If government labs and agencies of a rich nation cannot achieve this – who can?

(Part of this work has been presented before, at a pre-conference workshop to RDA20, Gothenburg, 2023)

How to cite: Pfeiffenberger, H. and Carlson, D.: Are Publicly Funded Data-Infrastructures Reliable?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20550, https://doi.org/10.5194/egusphere-egu25-20550, 2025.

EGU25-21042 | Posters on site | ESSI3.1

Efforts of the Small Bodies Node in Providing “Analysis Ready Data” to Support Open Science 

Eric E. Palmer, Kristina Lopez, and Mike Drum

The Planetary Data System (PDS) provides key structural support for Open Science by meeting the tenants of "Free, unrestricted access1.” Here we will discuss the need to expand our offerings by improving support for the OS tenants of "Ease of use.”

Analysis-ready data (ARD) provides data in formats that, while different than what was provided by the mission team, are orders of magnitude more useful to scientific researchers. 

For NASA Planetary Science Missions, the data is provided to us in stable and long-term formats that are well documented.  However, the data formats for each mission are typically different.  Additionally, many processing steps are not done by the science team for the archived products, such as ortho-rectification, geospatial positioning, or co-alignment with digital terrain models.  Additionally, there is little consensus within Planetary Science for a standard format for almost any data type, for example images that can be in FITS, VICAR, custom IMG formats, or sometimes JPEG.

PDS nodes have begun to host such ARD as either part of the official archive or outside of the archive using the new PDS annexes2.  We have several initiatives to support ARD.  These include the Small Bodies Image Browser and digital terrain models in both ISIS and GeoTiff formats. While generated data in these formats initially requires additional effort, once created they continuously provide value to the data user community.

Analysis-ready data can significantly increase "ease of use" in many different ways.  They typically will be preprocessed, saving data users significant effort that they would have spent learning how to process the data themselves. This preprocessing also lowers the technical barriers and eases the use of complex data sets. In addition to the preprocessing, datasets can be provided in standardized, commonly used data formats that are more useable and accessible than many of the current formats. Streamlining the ARD would greatly ease both researchers' and the public’s ability to use data spanning many different missions in ways that is not currently possible. Focusing on providing the most interoperable and usable data to the community also enables more interdisciplinary collaboration and increases reproducibility — all key goals of Open Science.  

Analysis-ready data in the PDS will be essential to create more open and usable data. As the complexity of planetary mission data increases, ARD can allow the PDS to maximize the scientific return of these valuable datasets.

References:
[1] NASA Science Mission Directorate. (2023). Open-Source Science Guidance, Version 2.1.
[2] Mouginis-Mark, P., Williams, D., Bleacher, J., et al. (2023). Analysis Ready Data (ARD) within the Planetary Data Ecosystem: Benefits for the Science Community. 54th Lunar and Planetary Science Conference.

How to cite: Palmer, E. E., Lopez, K., and Drum, M.: Efforts of the Small Bodies Node in Providing “Analysis Ready Data” to Support Open Science, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21042, https://doi.org/10.5194/egusphere-egu25-21042, 2025.

EGU25-21367 | Orals | ESSI3.1

AuScope’s Research Data Systems: Operationalising FAIR place-based research through collaboration 

Rebecca Farrington, Lesley Wyborn, Jo Croucher, Anusuriya Devaraju, Alex Hunt, Hannes Hollmann, Jens Klump, Angus Nixon, Alexander Prent, Sara Polanco, Nigel Rees, and Tim Rawling

Addressing global environmental and societal challenges requires robust, interdisciplinary data ecosystems that support collaboration across geographic, cultural, and disciplinary boundaries. AuScope, Australia’s National Research Infrastructure (NRI) provider for the geoscience community, collaboratively tackles interdisciplinary grand challenges such as climate change, natural resource security, and natural hazards. AuScope is funded by the Australian Government’s National Collaborative Research Infrastructure Strategy (NCRIS) and integrates tools, data, analytics, and services across Australian research and government agencies, in particular, partnering with organisations at the forefront of research data systems and infrastructure.

Through collaborations with CSIRO, Geoscience Australia, state and territory geological surveys, universities, and other NCRIS facilities, including the National Computational Infrastructure (NCI), the Terrestrial Ecosystem Research Network (TERN), and the Australian Research Data Commons (ARDC), AuScope is addressing the complexities of modern FAIR data management at scales ranging from small scale local installations to co-located High Performance Compute and Data (HPCD) Platforms. Key AuScope initiatives such as Geophysics 2030 Collections (https://ardc.edu.au/project/2030-geophysics-collections/), AusGeochem (https://ausgeochem.auscope.org.au/), the Modelling Atlas of The Earth (M@TE; https://mate.science), and the AuScope Data Repository (https://repository.data.auscope.org.au/) exemplify how the FAIR principles can be operationalised to support impactful research both within and beyond the geosciences and at multiple scales.

Nationally, AuScope collaborates with other Earth and Environmental Research Infrastructure providers, working to transform Australia’s research capabilities through, for example, Coastal Research Infrastructure (CoastRI) and implementing the National Digital Research Infrastructure Strategy (NDRI). Globally, AuScope contributes to initiatives like OneGeochemistry, the CODATA-led WorldFAIR Plus project, EarthScope (US), EPOS, Geo-INQUIRE, and ChEESE (Europe), ensuring compatibility with international research infrastructures, data standards, and best practices while at the same time, aligning with Australia’s geoscience priorities. 

This presentation will highlight how AuScope is progressively operationalising the FAIR and TRUST principles across its investments by focusing on place-based research to foster interoperability, strategic collaboration, and Open Science practices. By aligning with the CARE principles as well as advancing collaborative data infrastructure, AuScope creates trusted, interoperable data ecosystems that empower researchers to effectively and efficiently address pressing interdisciplinary societal challenges at both a national and international scale.

How to cite: Farrington, R., Wyborn, L., Croucher, J., Devaraju, A., Hunt, A., Hollmann, H., Klump, J., Nixon, A., Prent, A., Polanco, S., Rees, N., and Rawling, T.: AuScope’s Research Data Systems: Operationalising FAIR place-based research through collaboration, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21367, https://doi.org/10.5194/egusphere-egu25-21367, 2025.

EGU25-2295 | Orals | ESSI3.2

Data Lifecycle Management for Field Campaigns: Welcome to the Earth Observing Laboratory Field Catalog and Archive 

Jacquelyn C. Witte and the Data Management and Services Team

The NSF NCAR Earth Observing Laboratory (EOL) has supported over 600 national and international field campaigns which represent half a century of field-based observational science. Our mission is to provide responsive, high quality data services to researchers in field campaigns including pre-field phase planning, real-time decision-making tools, and long-term data curation to support the complete project life cycle. Such support includes (1) serving as the online hub for field campaign operations with access to real-time mission coordination displays and communication tools, (2) ensuring a secure, easily accessible archive of campaign observations, and (3) providing long-term stewardship and curation of observational datasets. All datasets in the EOL’s Field Data Archive are publicly accessible and findable at https://data.eol.ucar.edu/.  

 

EOL data management services are continuously evolving as we pursue FAIR and TRUSTed principles based on industry standards, user feedback and the desire to increase data discovery and accessibility to the broader scientific community. The management of our field campaign data is an iterative, human-driven and agile process. Thus, to address challenges arising from data preparation, preservation, and provenance metadata as the volume and variety of our data grows, EOL has developed tools and workflows that track and maintain the collection of data. In this presentation we will introduce highlights and functionalities of the Field Catalog and the Field Data Archive that together provide end-to-end customized data management services for field campaigns.

How to cite: Witte, J. C. and the Data Management and Services Team: Data Lifecycle Management for Field Campaigns: Welcome to the Earth Observing Laboratory Field Catalog and Archive, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2295, https://doi.org/10.5194/egusphere-egu25-2295, 2025.

EGU25-2803 | Orals | ESSI3.2

GOYAS: A FAIR-by-Design System for Innovative remote-sensing data products 

Fernando Aguilar Gómez, Verónica González-Gambau, Cristina González-Haro, Aina García-Espriu, Eva Flo, Estrella Olmedo, Isabel Caballero, Evgeniia Makarova, Marcos Portabella, Daniel García-Díaz, and Isabel Afán

The Geospatial Open Science Yielding Applications (GOYAS) project, under the umbrella of the Horizon Europe project “OSCARS”, proposes a new approach for open science and open data in remote-sensing, integrating FAIR principles (Findable, Accessible, Interoperable, and Reusable) from the initial design phase. GOYAS provides innovative and/or experimental Earth Observation (EO) data and open science practices to address diverse environmental challenges, delivering advanced geospatial products that are tailored to meet the needs of multiple stakeholders, including researchers, decision-makers, and environmental managers.

GOYAS focuses on generating innovative and accessible remote sensing products for a variety of applications: monitoring water quality parameters, such as turbidity or chlorophyll-a; deriving high-resolution bathymetric maps over coastal regions based on optical instruments; assessing oceanographic variables like sea surface temperature and salinity; improving ocean and atmosphere forecasting capabilities with enhanced sea-surface wind & stress products; and supporting ecosystem monitoring and management in protected areas such as Doñana National Park. These products are generated through the integration of multi-source EO data, including Copernicus Sentinel satellites and complementary datasets, with advanced processing pipelines built on machine learning algorithms and geospatial standards.

A core strength of the GOYAS project lies in its FAIR-by-design system architecture, which prioritizes:

  • Findability: Metadata-rich datasets indexed through open repositories and geospatial catalogues to enhance discoverability.

  • Accessibility: FAIR-compliant platforms with user-friendly interfaces that provide seamless access to data products, ensuring usability across diverse technical expertise levels. GOYAS aims at facilitating the access providing data in common formats and contextualizing them with proper metadata.

  • Interoperability: Adoption of open geospatial standards (e.g., OGC, INSPIRE) to ensure compatibility with existing systems and facilitate data exchange, specially under the context of Research Infrastructure hubs like ENVRI.

  • Reusability: Comprehensive documentation and adherence to open licenses that allow users to adapt and build upon project outputs.

Key innovations include the automated processing of remote-sensing data to extract actionable insights and the application of machine learning to improve the accuracy and reliability of derived parameters. For example, GOYAS employs advanced spectral analysis techniques to calculate shallow bathymetry with sub-meter precision in coastal environments, as well as algorithms for near-real-time detection of water quality anomalies in inland waters.

The system also provides support for the monitoring and management of sensitive ecosystems. In Doñana National Park, GOYAS enables the identification of changes in hydrological regimes or vegetation health through the integration of long-term EO datasets with local ecological studies. Similar applications extend to marine protected areas, where GOYAS aids in monitoring oceanographic dynamics and ecosystem responses to climate change.

This presentation will detail the design, architecture, implementation, and outcomes of the GOYAS project, emphasizing its alignment with FAIR principles and its transformative potential for environmental monitoring. By fostering interoperability and collaboration across disciplines, GOYAS serves as a model for how open science and advanced remote sensing can drive innovation, sustainability, and informed decision-making in geospatial research.

How to cite: Aguilar Gómez, F., González-Gambau, V., González-Haro, C., García-Espriu, A., Flo, E., Olmedo, E., Caballero, I., Makarova, E., Portabella, M., García-Díaz, D., and Afán, I.: GOYAS: A FAIR-by-Design System for Innovative remote-sensing data products, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2803, https://doi.org/10.5194/egusphere-egu25-2803, 2025.

EGU25-4203 | ECS | Orals | ESSI3.2

Escaping from the 1600s: Advancing FAIR scientific knowledge with reborn articles 

Lauren Snyder, Hadi Ghaemi, Ricardo Perez-Alvarez, and Markus Stocker

Text-based literature remains the primary expression of scientific knowledge. Since the first scientific article published in 1665, we have managed the switch from physically printed articles to PDFs, but nothing more. While PDF publications can be easily shared electronically, they remain unstructured text-based documents that machines cannot easily interpret (i.e., they are not machine-reusable). This limits our ability to use digital support tools to efficiently extract and organize knowledge from scientific articles. Rather, to reuse most scientific results (e.g., for synthesis research), we must first extract them from articles and organize them into databases, which is time consuming and prone to error. 

Here, we present reborn articles, which offer a novel approach to producing scientific knowledge. By integrating with programming languages commonly used for data analysis, like R and Python, reborn articles allow researchers to produce scientific results in a machine-reusable format from the outset. This means subsequent data users can download the results of a reborn article as a CSV file with just a click of a button and bypass post-publication data extraction. To support the production, publication, and reuse of reborn article data, we developed ORKG reborn, a FAIR knowledge online infrastructure. 

Using an ecological dataset, we showcase the production of a reborn article, and its impact on knowledge integration and synthesis. Building on the author’s original data analyses conducted in R, we developed an accompanying R script to produce machine-reusable descriptions of the original statistical models that were automatically harvested by ORKG reborn, eliminating manual data entry. We envision that the use of programming languages, like R, to facilitate the production of machine-reusable scientific knowledge could feasibly be streamlined into existing FAIR data management requirements that are already implemented by many academic publishers. Broad adoption of the approach across research communities could transform the way we share and synthesize scientific knowledge. 

How to cite: Snyder, L., Ghaemi, H., Perez-Alvarez, R., and Stocker, M.: Escaping from the 1600s: Advancing FAIR scientific knowledge with reborn articles, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4203, https://doi.org/10.5194/egusphere-egu25-4203, 2025.

EGU25-9401 | Orals | ESSI3.2

Scalable Solutions for Urban Data Spaces: Insight from the USAGE blueprint 

Piotr Zaborowski, Francesca Noardo, Giacomo Martiano, and Danny Vandenbroucke

The USAGE objective is to identify, implement, and demonstrate an architecture and solutions for a data space supporting the European Green Deal priorities. It implements the methodology based on the data USAGE data space framework built around specific use cases in the context of local and European policies and guidelines as well as digitalization agendas. Use cases, considered the primary value proposition for the data uptake, are developed and maintained in the USAGE framework. They cover  urgent municipalities scenarios like heat islands, clean energy, qir quality and mobility. Target requirements are translated into data and service requirements expressed in the ISO catalog-based model tailored to the specific data quality measures for the Decision Ready Information. Implementation of the value chain goes across various data inputs including satelite and airborne images, local sensors and citizen science data, surface and urban models producing intermediary and end user products and services. Disciplined and tool-supported collection of the data and application assets consistent with the INSPIRE-compliant schemas and data requirements model which allows them to leverage the solutions' potential and implement the value proposition for their providers. Profiled models create the frames of the data value chain, documenting processing steps from the data requirements through BPMN data flow models linking to the used and produced assets. In addition, licensing schema, including the constraints model, allows for data sovereignty and trust among the data space actors.

The outcome blueprint for the urban data space goes beyond the USAGE pilots to test scalable solutions based on adopting the proposed set of standards coming mainly from ISO, OGC, W3C, OASC and their extensions. It is built in the European initiatives and legal references (i.e., the European strategy for data, the European interoperability framework, the European interoperability reference architecture), and reviewed several projects and initiatives results contributing to shaping data spaces: Open DEI design principles, the International Data Spaces Association (IDSA) reference architecture, Gaia-X architecture, Data Spaces Business Alliance (DSBA) documents, the Data Spaces Support Centre (DSSC) results, Data Space for Smart and Sustainable Cities and Communities (DS4SSCC) outcomes, and the GREAT project Technical Blueprint. Presentation goes across the best practices and guidances extracted from the implementation of the FAIR dataspace and considerations given defined frameworks.

How to cite: Zaborowski, P., Noardo, F., Martiano, G., and Vandenbroucke, D.: Scalable Solutions for Urban Data Spaces: Insight from the USAGE blueprint, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9401, https://doi.org/10.5194/egusphere-egu25-9401, 2025.

EGU25-9739 | Posters on site | ESSI3.2

Reducing the Pain of Data Discovery in Earth System Science 

Aenne Loehden, Claudia Martens, and Andrea Lammert

Ontologies offer significant potential for advancing Earth System Science (ESS) by improving the discoverability and usability of complex datasets and tools. This poster builds on last year’s comic, which illustrated the foundational benefits of ontologies, and presents the first steps in implementing generic tools from already existing terminology services designed to enhance data findability and data comprehension. These tools enable scientists to easily search for appropriate data and retrieve information about data from specific repositories, thus supporting the FAIR (Findable, Accessible, Interoperable, and Reusable) principles in ESS.

Key aspects of terminologies include the clear and consistent description of scientific terms, their relationships, and the unambiguous identification of terms to prevent inconsistencies. By using terminologies we can ensure that terms are defined in a way that is both standardized and interoperable across different datasets and research communities. Concrete examples will be drawn from the World Data Center for Climate (WDCC), where first steps have been taken to implement generic tools and extend the application of terminologies, and to thus enhance data discoverability and facilitate better searchability of climate-related information.

How to cite: Loehden, A., Martens, C., and Lammert, A.: Reducing the Pain of Data Discovery in Earth System Science, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9739, https://doi.org/10.5194/egusphere-egu25-9739, 2025.

EGU25-10627 | Orals | ESSI3.2

FAIR EU soil vocabularies: an overview of joint efforts from some EU Soil Mission projects 

Mickaël Beaufils, Paul van Genuchten, Fenny van Egmond, and Kathi Schleidt

Vocabularies or thesauri, lists of terms with their definitions and unique ID, like a dictionary of a language, play a critical role in the domain of soil science, providing a standardized framework for accurately documenting and communicating soil characteristics. In soil science, the use of precise and consistent terminology ensures the effective exchange of data, promoting interoperability among researchers, practitioners, and decision-makers. A well-structured vocabulary, part of soil classification or soil description standards, facilitates the classification of soil properties, such as texture, structure, fertility, and organic content, allowing combining data from different sources but described in a similar way. And thereby enabling reliable comparison and interpretation across different regions and time periods. Furthermore, these vocabularies enable and support the development of standardized databases, soil datasets and soil monitoring systems, which are essential for environmental management, land use planning, and agricultural practices. Inaccurate or ambiguous soil descriptions can lead to misinformed decisions, making the establishment of clear, universally accepted vocabularies crucial for advancing soil science, conservation efforts, and sustainable land management practices. Such practices would greatly enhance the FAIRness of the data being managed, ensuring data conservation over time.

Soil vocabularies come from many sources, some national or regional, some from international organizations such as the Food and Agriculture Organization of the United Nations (FAO) or the International Union of Soil Sciences (IUSS), e.g. World Reference Base for Soil Resources (WRB) or FAO Guidelines on Soil Description. Several initiatives worked on the identification and provision of agreed vocabularies in order to ensure the interoperability of their results at different scales (national, EU, international). This includes work by standard setting organizations (eg. ISO TC190), legislation (eg. EU INSPIRE Directive) and of course numerous collaborative projects, such as SIEUSOIL, EJP SOIL, ISLANDR, SoilWise, SPADES, Soil Mission Support and MARVIC. At present, many existing vocabularies have not been exposed in a referenceable and machine-readable manner, and instead remain “trapped” within PDF documents. Extracting the relevant concepts and exposing them in both human and machine readable forms on persistent URIs would be a valuable step towards soil data harmonization.

The European Mission: A Soil Deal for Europe, with currently about 50 research projects and a network of 100 living-labs and lighthouses, offers an interesting environment and opportunity for the co-creation of a harmonised framework for soil vocabulary description. Due to the diversity of Soil Mission Projects, gaps in existing vocabularies can be identified and experience can be gained in how to best present vocabularies for both data annotation as well as data discovery.

In this presentation we will share the current status on this topic, offering a non-exhaustive yet hopefully informative overview on existing materials (vocabularies and associated technologies to share them), on-going work and key challenges for achieving better soil data interoperability.

This study was made possible through funding from the EU's Horizon Europe program, specifically the ISLANDR and SoilWise projects.

How to cite: Beaufils, M., van Genuchten, P., van Egmond, F., and Schleidt, K.: FAIR EU soil vocabularies: an overview of joint efforts from some EU Soil Mission projects, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10627, https://doi.org/10.5194/egusphere-egu25-10627, 2025.

EGU25-11467 | ECS | Posters on site | ESSI3.2

Advancing FAIR geochemical data: 25 Years of GEOROC database service 

Leander Kallas, Marthe Klöcking, Kirsten Elger, Bärbel Sarbas, Adrian Sturm, Stefan Möller-McNett, Matthias Willbold, and Gerhard Wörner

The GEOROC synthesis database, a pioneering open-access resource for geochemical and isotopic data, marks 25 years of service to the geoscience community. Over its history, GEOROC has compiled data from more than 22,750 publications in the field of geochemistry, and provides free access to over 39 million individual data values, primarily on igneous and metamorphic rocks, minerals and their inclusions. As a cornerstone for interdisciplinary research, GEOROC is complementary to other geochemical synthesis databases like PetDB, AstroMat and GeoReM, in facilitating reuse of data for innovative studies that leverage data analytics and machine-learning approaches across geoscientific disciplines and beyond.

The Digital Geochemical Data Infrastructure (DIGIS) project for GEOROC 2.0 is providing an up-to-date IT infrastructure that aligns GEOROC with the FAIR principles. Data findability and accessibility are ensured through the newly developed API and the improved GEOROC web interface that allows users to retrieve a variety of distinct data products and services, including a fully customizable search functionality. Interoperability is achieved via implementation of a feature-based data model compatible with the OGC Observations and Measurements standard and controlled, machine-readable vocabularies that harmonize geospatial, analytical and sample-related metadata, and enabling seamless integration in multiple databases and portals (e.g., EarthChem). Reusability is further supported by archiving time-stamped GEOROC data products in the DIGIS Data Repository, hosted by GFZ Data Services, where datasets with digital object identifiers (DOIs) are archived for the long-term. Additionally, researchers are encouraged to directly submit new or already “published” datasets to this domain repository—through standardized (meta-)data templates, ensuring high-quality data submissions that facilitate data quality assessment and reuse.

In collaboration with national and global initiatives, such as OneGeochemistry and NFDI4Earth, the DIGIS project further promotes practical approaches to the FAIR principles for geochemistry by developing unified controlled vocabularies for geochemical data and their metadata (e.g., analytical methods, sample description, location). These vocabularies also integrate external standards, such as the International Mineralogical Association’s "List of Minerals" and MinDat’s "Subdivisions of Rocks," alongside newly developed (and published) frameworks for categories such as geological setting and analytical methods (collaboration with EarthChem). By harmonizing metadata across geospatial, analytical and sample-related categories, these efforts ensure consistency, improve data quality assessment and control and enhance interoperability across data systems, including but not limited to GEOROC, PetDB, and AusGeochem. Such advancements expand the potential applications of geochemical data, fostering innovation in fields such as environmental science, remote sensing, archaeology and geohealth.

With 25 years of experience and ongoing innovation through the DIGIS project, the GEOROC database exemplifies how operationalizing the FAIR principles enhances its value as a critical resource for the geoscience community. By providing both FAIR and open data, GEOROC empowers researchers to conduct reproducible, impactful studies and fosters interdisciplinary collaboration, driving innovation and advancing progress across the geosciences.

How to cite: Kallas, L., Klöcking, M., Elger, K., Sarbas, B., Sturm, A., Möller-McNett, S., Willbold, M., and Wörner, G.: Advancing FAIR geochemical data: 25 Years of GEOROC database service, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11467, https://doi.org/10.5194/egusphere-egu25-11467, 2025.

EGU25-14320 | ECS | Orals | ESSI3.2

EarthBank by AuScope: Building FAIR research data infrastructure for the global geochemical community 

Angus Nixon, Bryant Ware, Brent McInnes, Fabian Kohlmann, Moritz Theile, Wayne Noble, Yoann Gréau, Hayden Dalton, Halimulati Ananuer, Malcolm McMillan, and Ashley Savelkouls

The geochemical community increasingly generates and requires large volumes of analytical data from a wide array of acquisition methods, analytical scales, and sample types in order to address broad research applications. Resulting datasets are commonly collected and reported through non-standardised protocols and reporting formats, if indeed standards are applied at all, which inhibits easy sharing of data during collaborative research projects or repurposing of legacy data. Existing repository services do not presently satisfy requirements for Findable, Accessible, Interoperable and Reusable (FAIR) data, and especially contain significant flaws as to the reuse and interoperability of geochemical data. Generalist repositories such as Zenodo or Figshare do not provide consistent data structures or curation, hence data held within these services is highly variable with regard to format, parameters reported and potentially quality. While domain repositories commonly do implement internally consistent data formats and a level of curation, data within repositories is gathered from published sources which may be incomplete or unstructured, and hence often lack the complete information (metadata) required to appropriately describe the data and allow it to be confidently reused. 


To truly unlock the potential of the ever expanding wealth of geochemical data and meet FAIR requirements, improvements to the data infrastructure landscape are clearly required. The AuScope Geochemistry Network (AGN) is an Australian-based collaboration of geoscientists producing bespoke data resources and infrastructure for the international community to capture, normalise, and share geochemical data resources. These resources include best practice data reporting schema and vocabularies for a variety of data types, produced through collaborations with expert advisory groups and, where available, following or expanding on existing international community recommendations. These data resources have been implemented to the EarthBank platform (formerly AusGeochem), an open web service designed by the AGN to capture, share, store and evaluate geochemical data and metadata. Unlike many other services, researchers are able to upload data prior to publication which can assist both in allowing researchers to compare their data with other existing resources prior to submission, but importantly also improves the likelihood of capturing the full data and metadata associated with analyses required for reuse. Once data is uploaded to this service it may be associated with a dataset DOI to support data access requirements for publication, in order to streamline the publication process and provide a domain specific repository for supplemental data. Data models for U/Pb, fission track, (U-Th-Sm)/He, 40Ar/39Ar and inorganic major and trace geochemistry data types are presently implemented within EarthBank, allowing users to freely upload generated research data for these systems, or explore and integrate existing datasets. Best practice templates for upload are openly available through the EarthBank platform, and vocabularies are openly discoverable through the Research Vocabularies Australia (RVA) service. These resources may be used not only to upload data, but also to develop cross-walks for machine-to-machine interoperability with other repository services to build a global FAIR compliant infrastructure required to maximise data access and improve research outcomes.

How to cite: Nixon, A., Ware, B., McInnes, B., Kohlmann, F., Theile, M., Noble, W., Gréau, Y., Dalton, H., Ananuer, H., McMillan, M., and Savelkouls, A.: EarthBank by AuScope: Building FAIR research data infrastructure for the global geochemical community, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14320, https://doi.org/10.5194/egusphere-egu25-14320, 2025.

EGU25-14828 | Orals | ESSI3.2

Uplifting and streamlining FAIR data implementation for Australia’s climate modelling outputs 

Kelsey Druken, Clare Richards, Romain Beucher, Johanna Basevi, Chris Bull, Claire Carouge, Martin Dix, Aidan Heerdegen, Paul Leopardi, Davide Marchegiani, Heidi Nettelbeck, Anton Steketee, Charles Turner, Marc White, and Spencer Wong

Australia’s Climate Simulator (ACCESS-NRI) is a national research infrastructure established to support the Australian Community Climate and Earth System Simulator (ACCESS) modelling system. Since its launch in 2022, ACCESS-NRI has focused on modernising climate modelling software and data practices for ACCESS. Guided by the needs of our community, our goal is to make the modelling framework and data outputs more FAIR (Findable, Accessible, Interoperable, and Reusable) and easier to use.  

One of the key challenges in achieving FAIR for ACCESS data is the reliance on often optional post-processing steps to meet most of the FAIR guidelines. While ACCESS model outputs generally follow community standards (e.g., CF-Conventions), their implementation can be inconsistent across modelling components (e.g., atmosphere, ocean, and land models) as well as among individual data generators. As a result, using direct model output data frequently requires users to have previous knowledge and understanding of the specific climate models and leads to significant overheads for compatibility with data discovery and evaluation tools (e.g., Intake, ESMValTool). 

As a new infrastructure dedicated to Australian climate software and data, ACCESS-NRI has a unique opportunity to uplift and directly embed FAIR practices into the climate modelling software components we maintain and support. Building on successes and lessons learned from participation in global intercomparison activities such as CMIP6, ACCESS-NRI is working to apply similar data standardisation practices for the lower-level model outputs in a way that enhances consistency and usability. The effort involves close collaboration with the research community, identifying gaps and commonalities to establish a data specification that can be versioned and linked to future ACCESS model releases. This includes minimum and recommended requirements for file and dataset metadata such as: controlled vocabularies, file and variable naming conventions, provenance statements, and other critical elements to ensure data consistency and usability across all ACCESS components.    

By embedding FAIR principles directly into the ACCESS modelling system, ACCESS-NRI is not only addressing current challenges but is also future-proofing Australia’s climate modelling capabilities to meet the evolving needs of the research community. This approach will make data and tools more accessible, reduce research overheads, and enhance the adaptability of the infrastructure to future changes and new technologies. 

How to cite: Druken, K., Richards, C., Beucher, R., Basevi, J., Bull, C., Carouge, C., Dix, M., Heerdegen, A., Leopardi, P., Marchegiani, D., Nettelbeck, H., Steketee, A., Turner, C., White, M., and Wong, S.: Uplifting and streamlining FAIR data implementation for Australia’s climate modelling outputs, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14828, https://doi.org/10.5194/egusphere-egu25-14828, 2025.

EGU25-16485 | Orals | ESSI3.2

Improving the accessibility of ECMWF open weather forecast data and charts: maintenance challenges 

Milana Vuckovic, Emma Pidduck, Cihan Sahin, and Iain Russell

ECMWF's move towards an extensive free and open data policy is approaching its final phase, extending its user base far beyond operational forecasters in Member and Co-operating States and other licensed customers. Beginning in 2020, the first phase saw the opening of hundreds of web forecast charts (www.charts.ecmwf.int) and made archived data available under a Creative Commons (CC BY 4.0) open licence. This transition continued in January 2022 with the introduction of a free and open subset of real-time forecast data, with ongoing updates incorporating new parameters and datasets. Notably, the latest updates in 2024 included increasing the resolution from 0.4° to 0.25° and including the new Artificial Intelligence Forecasting System (AIFS) forecast data.
This phased move towards free and open data supports the UN EW4All initiative and also aims to support creativity, innovation and reproducibility in scientific research and weather applications. However, this can not be achieved by only opening the real time and archived data. The users need to be able to find and easily use the data and integrate it into their own research work or application workflows.
To address this, additional efforts are underway to improve the data's FAIR (Findable, Accessible, Interoperable and Reusable) attributes. Key developments include the creation of open source Python libraries for data downloading, processing and visualisation under the EarthKit umbrella, alongside the introduction of a set of Jupyter notebooks, each of which is reproducing one open weather forecast chart - from the downloading the data to processing and visualisation.
However, the tools and data constantly change, and keeping up with these changes in the example Jupyter notebooks presents a significant challenge if not designed with the maintenance in mind.
This talk will provide an overview of the open forecast web charts and the use of Jupyter notebooks for their reproduction, followed by an exploration of the maintenance challenges and future plans.

How to cite: Vuckovic, M., Pidduck, E., Sahin, C., and Russell, I.: Improving the accessibility of ECMWF open weather forecast data and charts: maintenance challenges, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16485, https://doi.org/10.5194/egusphere-egu25-16485, 2025.

EGU25-19266 | Posters on site | ESSI3.2

Establishing FAIRness through all-actor approaches to data pipelines: Frameworks for successful development of data standards and pipelines at the UK’s National Centre for Atmospheric Sciences 

Graham Parton, Barbara Brooks, Wendy Garland, Joshua Hampton, David Hooper, Nicholas Marsden, Hannah Price, Hugo Ricketts, Dave Spronson, Ag Stephens, and Chris Walden

The FAIR data principles are a common theme in many discussions and focus of work within research data management. Such work often focuses on particular parts of the data management lifecycle, for example: FAIR through data management planning, FAIR through data discovery and, more recently, areas of FAIR as applied to software and machine learning. 

However, whilst there are many successful attempts at enhancing metadata and data FAIRness for specific parts of the data lifecycle, there may be issues that only arise when considering the overall interconnections between the various stages and the associated actors. For example, a domain may follow common file and metadata conventions for data interoperability, such as CF conventions, enabling research to take place utilising multiple data sources, but pertinent metadata to long-term curation or wider end-usability may not be presented or indeed captured at source. This can have ongoing issues around the level that wider (true?) FAIRness that can be reached and present additional overheads for other actors wishing to handle such data resources, such as manual effort needed for full long-term curation or missed opportunities for data re-use in other spheres.

Recognising these issues and, crucially,  the interplay between all actors along the data lifecycle, the UK’s National Centre for Atmospheric Science (NCAS) have developed the frameworks to ensure all actors’ needs are considered. These are succinctly captured in the ‘NCAS Data Pyramid’, where each corner represents a given actor (data provider, long-term archive, those creating tools aiding data flows and utilisation, end-user community), whilst the sides explore the interconnections between these actors. All parts of the pyramid (corners and sides) provide a range of use-cases and requirements that need to be supported. This approach has enabled NCAS to then develop a range of data standards to enhance data FAIRness for surface and remote sensing data (including from ships and aircraft), imagery data and, in due course, laboratory data.

Furthermore, to aid establishing new data standards NCAS has developed data standards development framework, utilising the ‘Scope -> Define -> Develop -> Sustain’ data standard lifecycle:

  • Scope: Identify community groups. Assess their needs. Determine the scope for the standard.
  • Define the standard by: ensuring all stakeholder needs are covered; defining user-focused data products that it will deliver; and the underpinning standards to be drawn on for wider interoperability. 
  • Develop: provider tools (including checkers for compliance); data delivery pipelines (including those workflows to capture internal/external metadata required for data use/contextualisation of data (e.g. project info); develop end-user data exploitation(visualisation) tools
  • Sustain: having developed standards and workflows have a governance structure to maintain and manage future iterations of the standards development cycle. This must ensure that it refers back to the community groups (as in step 1). 

The approach also keeps wider inter-standards interoperability a key focus throughout. The success of this approach is demonstrated through the establishment of data pipelines aiding data to flow with associated metadata from provider to end-user and has seen wider adoption of NCAS data standards within the wider atmospheric community.

How to cite: Parton, G., Brooks, B., Garland, W., Hampton, J., Hooper, D., Marsden, N., Price, H., Ricketts, H., Spronson, D., Stephens, A., and Walden, C.: Establishing FAIRness through all-actor approaches to data pipelines: Frameworks for successful development of data standards and pipelines at the UK’s National Centre for Atmospheric Sciences, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19266, https://doi.org/10.5194/egusphere-egu25-19266, 2025.

EGU25-19487 | Orals | ESSI3.2 | Highlight

Challenges and opportunities in implementing open and FAIR data in Intergovernmental Panel on Climate Change (IPCC) Seventh Assessment Report (AR7)  

Xiaoshi Xing, Gian Carlo Delgado Ramos, Azra Alikadic, April Lamb, Martina Stockhause, Lina E. Sitz, and Adam Milward

Intergovernmental Panel on Climate Change (IPCC) authors of assessment reports (ARs) and special reports (SRs) use a huge volume of input data, generate a great deal of intermediate data in the process, and produce a large amount of final data for figures and annexes in the published reports. In previous assessment cycles before the Sixth Assessment Report (AR6), only a limited amount of IPCC data were archived and made publicly available. There was  great progress in the AR6, but many critical data sets were still not properly curated. This resulted in a data rescue effort during the transition from AR6 to AR7, supported by the IPCC and government fundings. The challenges encountered during the data rescue effort included missing or lost data after the report publication, missing data licensing agreements, version control issues, and missing data quality assurance/quality control (QA/QC) so that some data did not match the published figures. Addressing these issues demanded significantly more resources than the regular process to track, retrieve, archive, and resolve the legal and technical issues.

In the Seventh Assessment Report (AR7), IPCC progressively promotes the FAIR data principles (Findable, Accessible, Interoperable, and Reusable) through the IPCC Task Group on Data Support for Climate Change Assessments (TG-Data) and the Data Distribution Centre (DDC) (1, 2). The Working Group Technical Support Units (TSUs) have also designated data specialists in the TG-Data (3). This provides opportunities to support authors in implementing open and FAIR data in IPCC AR7. For example, in Chapter 2 of the Special Report on Climate Change and Cities (SRCities), there is an area of focus on “Data, information, tools accessibility/availability/usability/transparency" (4). By collaborating the TSUs and DDC can provide a coordinated approach that supports authors with training and tools on data workflow, metadata schema, data provenance, licensing and citation, persistent identifiers, etc., to improve the data curation process and to avoid the issues encountered in previous cycles.

References:

  • 1. Intergovernmental Panel on Climate Change. (2023). TG-Data Recommendations for AR7 (1.0). Zenodo. https://doi.org/10.5281/zenodo.10059282
  • 2. Stockhause M, Huard D, Al Khourdajie A, Gutiérrez JM, Kawamiya M, Klutse NAB, Krey V, Milward D, Okem AE, Pirani A, Sitz LA, Solman SA, Spinuso A, Xing X. (2024).  Implementing FAIR data principles in the IPCC seventh assessment cycle: Lessons learned and future prospects. PLOS Climate 3(12): e0000533. https://doi.org/10.1371/journal.pclm.0000533
  • 3. https://www.ipcc.ch/data/ (2025)
  • 4. IPCC Special Report on Climate Change and Cities (SRCities) report outline. (2024). https://www.ipcc.ch/site/assets/uploads/2024/08/IPCC-61_decisions-adopted-by-the-Panel.pdf

How to cite: Xing, X., Delgado Ramos, G. C., Alikadic, A., Lamb, A., Stockhause, M., Sitz, L. E., and Milward, A.: Challenges and opportunities in implementing open and FAIR data in Intergovernmental Panel on Climate Change (IPCC) Seventh Assessment Report (AR7) , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19487, https://doi.org/10.5194/egusphere-egu25-19487, 2025.

EGU25-19699 | Orals | ESSI3.2

Building an EOSC based virtual research environment to support the adoption of FAIR and Open Science practices in Climate Change Adaptation communities 

Raúl Palma, Malgorzata Wolniewicz, Adam Rynkiewicz, José Manuel Gómez, Andres Garcia Silva, Daniel Garijo, Esteban Gonzalez Guardia, and Anne Fouilloux

During the last years, Open Science has been gaining increasing attention from research communities and policy makers because of the benefits it can provide not only to scientists, but also to society in general, as it can accelerate the production of science and the quality of results. Open science is a policy priority for the European Commission (EC) and the standard method of working under its research and innovation funding programmes. Thus, the EC initiated the European Open Science Cloud (EOSC) initiative, which aims to create a virtual environment for sharing and accessing research data across borders and scientific disciplines, aligning with Open Science and FAIR principles. EOSC specified a layered approach with a set of core services at its center, a federated data layer, a rich set of exchange services to expand the capabilities offered to researchers across disciplines, plus a set of thematic/discipline-specific services. To fully realise EOSC’s vision, it is envisioned as a federation of distributed systems, combined into a system of systems, consisting of multiple Nodes’. At the end of last year, the first of such nodes (EOSC EU node) was launched featuring the core services enabling scientific research infrastructures to federate and a set of common exchange “horizontal services” for end-users to benefit from. 

Based on the integration of thematic, horizontal, and core resources, the goal is that EOSC enables the creation of thematic execution environments/VREs. A VRE is an online support system for researchers,  encompassing online tools, network resources and technologies interoperating with each other to ease/enhance the research process within and across institutional boundaries, facilitating collaboration, data management, analysis, and other research-related activities in one online space.

To build an EOSC-based VRE, we have leveraged and integrated different core and exchange services. At the center of the proposed VRE are RO-Crate based research objects (providing an implementation of the FAIR digital object), as well as the associated technological support (provided by ROHub platform), to manage the research lifecycle and the associated scientific resources used and produced. The VRE leverages data cubes services for efficient and scalable structured data access and discovery, AI-based text mining services  that extract machine-readable metadata from scientific resources supporting recommendations and comprehension analysis, and FAIR assessment tools supporting researchers in the FAIRification of their outcomes. Additionally, the VRE relies on EOSC services for authentication and authorization to enable seamless access to different services, the computing platforms to execute computational methods, and data repositories to store and/or share their data in their personal/community workspaces or general repositories. The VRE also connects DMP platforms to enable the creation of machine-actionable plans, and with the scientific knowledge graph to enable the discovery of resources by different communities. In the FAIR2Adapt project, such environment is being enhanced with a set of added-value services (e.g., search and discovery using NL questions, multilingual semantic enrichment, sentence detection, FAIRness-aware search and recommendations, and multilingual generative question answering) and adapted to boost FAIR adoption in Climate Change Adaptation communities and research.

How to cite: Palma, R., Wolniewicz, M., Rynkiewicz, A., Manuel Gómez, J., Garcia Silva, A., Garijo, D., Gonzalez Guardia, E., and Fouilloux, A.: Building an EOSC based virtual research environment to support the adoption of FAIR and Open Science practices in Climate Change Adaptation communities, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19699, https://doi.org/10.5194/egusphere-egu25-19699, 2025.

Assessing the status and trends of water quality in inland water bodies requires access to reliable water quality monitoring data and associated metadata such as the monitoring locations, sampling methods, monitoring equipment and analytical methods. Many environmental agencies and research organizations collect water quality monitoring data, but unlike in other environmental domains and due to a lack of common best practices and standards, most organizations use their own data models, formats and controlled vocabularies to store and share these data. As a result, large-scale water quality analyses with a transboundary, continental or global scope require significant efforts to collect the necessary monitoring data from different sources and to harmonize the different data structures. Several international initiatives such as the UNEP Global Environment Monitoring System for Freshwater (GEMS/Water)1 or research activities such as the Global River Water Quality Archive (GRQA)2 have compiled global water quality datasets to facilitate large-scale hydrological studies, all facing the same challenges and often duplicating data processing efforts.
Over the last 20 years, the observing community has developed data models and semantic ontologies such as the OGC Observations, Measurements, and Samples (OMS)3 standard or the OGC/W3C Semantic Sensor Network (SSN)4 ontology to describe observations and associated metadata. These form the basis of several standards for the exchange of hydrological observation data such as the WaterML 2.0 family of standards. However, water quality specific aspects such as the description of sampling activities and associated metadata have not yet been included in these water specific standards. 
To address this issue, several government agencies and research organizations have started a Water Quality Interoperability Experiment (WQIE) within the Open Geospatial Consortium (OGC) in 2022. Several use cases for the exchange of water quality monitoring data of physical and chemical parameters monitored in surface and groundwater bodies using in-situ (sensor) or ex-situ (laboratory) monitoring were developed and described as object diagrams in UML based on the OMS conceptual model. Based on this exercise, a physical data model was developed by extending the OGC SensorThingsAPI (STA)5 with a plugin for the open source FROST server6. Several WQIE participants deployed pilot instances of water quality enabled FROST servers, making their water quality data publicly available. A web client was developed to facilitate access to the various STA endpoints and to enable data visualisation7
This presentation will give an overview of the developments of the OGC Water Quality Interoperability Experiment, highlighting achievements, outstanding challenges and future development plans. 

References:

1 https://www.unep.org/explore-topics/water/monitoring-water-quality

2 Virro, H., Amatulli, G., Kmoch, A., Shen, L., and Uuemaa, E.: GRQA: Global River Water Quality Archive, Earth Syst. Sci. Data, 13, 5483–5507, https://doi.org/10.5194/essd-13-5483-2021, 2021.

3 https://docs.ogc.org/as/20-082r4/20-082r4.html

4 https://www.w3.org/TR/vocab-ssn/

5 https://www.ogc.org/publications/standard/sensorthings/

6 https://github.com/hylkevds/FROST-Server.Plugin.WaterQualityIE/tree/main

7 https://api4inspire.k8s.ilt-dmz.iosb.fraunhofer.de/servlet/is/226/ 

How to cite: Heinle, M. and Saile, P.: A step towards FAIR water quality data – lessons learned from the OGC Water Quality Interoperability Experiment, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19719, https://doi.org/10.5194/egusphere-egu25-19719, 2025.

Since their development, the FAIR principles have been met with broad acceptance in the scientific community. Tools based on various approaches are available to assess the FAIRness of individual data sets. These range from qualitative assessments based on questionnaires to automated quantitative measurements of fairness. As the FAIR principles are rather vaguely formulated, these approaches are based on individual, often differing, interpretations of the FAIR principles. In addition, the authors of the FAIR principles explicitly recognize the different implementations of FAIR within the various specialist communities. This makes it necessary to develop community-specific metrics and tests and to adapt FAIR assessment tools accordingly.

This diversity of methods for assessing FAIR is encouraging, as it sheds light on a variety of aspects of FAIR. However, this also sometimes leads to different, divergent results from these tools, which is difficult for users to work with. In addition, the measurement of FAIRness of individual datasets is heavily dependent on various technical implementations on the part of the data providers and their service providers. Numerous, possibly unintentional restrictions on the accessibility of datasets can influence or falsify FAIR measurements. 

In this presentation, we would like to report on our experiences with the applied FAIR assessment within this context. We will report on the further development of F-UJI, in particular our experiences with discipline-specific FAIR metrics and their implementation. Furthermore, we will discuss the limitations of FAIR measurements and try to delineate FAIR from aspects of data quality and accessibility and how to derive informative holistic assessments of datasets that include all these aspects in the future.

How to cite: Huber, R.: Opportunities and limitations of applied FAIR evaluation of data sets, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20064, https://doi.org/10.5194/egusphere-egu25-20064, 2025.

EGU25-20123 | Orals | ESSI3.2

Automatic annotation following the I-ADOPT framework 

José Manuel Gómez Pérez and Andrés García

The fulfillment of the FAIR principles is a central requirement in modern research. Data findability and reusability are highly dependent on the quality and interoperability of their metadata. Among other attributes in earth and environmental sciences, FAIR metadata should ensure consistent and uniquely referenceable naming of geoscientific variables that support machine-interpretable semantic annotations. But in practice, most terminologies used to describe datasets and observed variables vary wildly in their granularity, quality, governance and interconnectivity which, in turn, limits their interoperability. The RDA endorsed I-ADOPT Framework addresses this issue by breaking down descriptions of observed variables into five well-defined atomic components ObjectofInterest, Property, Matrix, Constraint and Context anticipating their annotation with generic terms from FAIR semantic artefacts. As of today, the I-ADOPT decomposition is still a highly manual process that requires semantic and domain skills. Here, we propose the application of Large Language Models (LLM) to transform scientific terms into I-ADOPT-aligned descriptions. This model will enable the transformation into machine-interpretable representations by simply using natural language descriptions of observational research provided by domain experts. We will leverage the existing set of high-quality, human-made formalizations of I-ADOPT variables to adjust the LLM for this task. We will consider LLM in zero-shot scenarios where the LLM is used in its pretrained version and in-context learning where the LLM sees some examples of the task. We will also consider training specialist LLM where the LLM is further fine-tuned for this task, although the success of this approach depends on the amount of training data available. For developing this model and a first demonstrator, we will build on our previous experience in developing the I-ADOPT Framework, in transfer learning and fine-tuning neural networks, FAIR data stewardship, research data infrastructures and research software engineering. Our project will be further linked to several other ongoing activities and initiatives both on a national and also European level, which allows us to directly evaluate the performance of our LLM by potential end-users and communities. Such a service will be integrated into platforms like RoHub to help scientists make research datasets FAIR.

How to cite: Gómez Pérez, J. M. and García, A.: Automatic annotation following the I-ADOPT framework, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20123, https://doi.org/10.5194/egusphere-egu25-20123, 2025.

EGU25-20132 | Orals | ESSI3.2

How domain repositories support reusable data: metadata tools from GFZ Data Services 

Marcel Meistring, Holger Ehrmann, Jana Franz, Simone Frenzel, Ali Mohammed, and Kirsten Elger

The availability of reusable data and their associated metadata is increasingly demanded to address global societal challenges. Research data repositories and databases are the primary access points for geosciences data, and especially domain repositories are known to publish well documented and reusable data. This is due to a thorough data and metadata curation provided by the repository staff that usually includes domain scientists. Overall, the documented publication of a complex data set via a domain repository often takes time and additional preparation by the scientists, but the results clearly show a significant increase of the metadata and data quality, including the provision of cross-references to other publications, datasets, code and originating physical samples.

The largest challenge for domain repositories is to provide incentives to the researchers that reduce their workload and in the same time ensure a high quality of metadata and data documentation already at an early stage of a planned data publication. This challenge is especially high in repositories with a focus on the highly variable and usually small data from so-called “long-tail communities”. GFZ Data Services is a domain repository for DOI-referenced geosciences data and scientific software, hosted at the GFZ Helmholtz Centre for Geosciences. The repository has both a focus on the curation of long-tail data, and offers data publication services for international projects and services in the geosciences. To support researchers with the provision of descriptive metadata and receive structured data documentation, GFZ Data Services has developed an online metadata editor and data description templates. This presentation will focus on these support tools and demonstrate how both help the researchers and in the same time reduce the data curation workload.

A major focus will lay on our new metadata editor that is currently jointly developed between the University of Applied Sciences Potsdam and GFZ Data Services. The new metadata editor will enhance the support of users in data entry, so that the manual curation effort by the GFZ Data Services is reduced, and the metadata quality is improved at the same time. Technically, it has a responsive design and offers a dark mode. New facets include the ability to retrieve specific information, e.g., affiliations from the ROR API via a dropdown menu. Keywords are made uniquely identifiable through the automatic storage of schema names and uniform resource identifiers of the specific terms. All integrated thesauri can be updated via API calls. Real time validation of the input fields prevents the submission of incomplete or incorrect entries, so that significantly less work is required in data curation. The integrated help guide supports users to fill in the input fields.

The data description templates collect additional technical description in a structured form and are essential for data reuse. They are available in “commented” and “usable” versions and ensure that the descriptions meet our requirements (for many researchers the data documentation is new), offer clear instructions and even reduce the workload of the curators, because the descriptions are already provided at a very high level of content.

How to cite: Meistring, M., Ehrmann, H., Franz, J., Frenzel, S., Mohammed, A., and Elger, K.: How domain repositories support reusable data: metadata tools from GFZ Data Services, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20132, https://doi.org/10.5194/egusphere-egu25-20132, 2025.

The Intergovernmental Panel on Climate Change (IPCC) Data Distribution Centre (DDC) serves as a critical registry for climate change data, providing a shared infrastructure to ensure data quality and accessibility for the scientific community. Managing data to support IPCC reports presents challenges due to its multidisciplinary nature and diverse sources.

Key to this effort is the curation of metadata, particularly developing a metadata schema that enables data to be FAIR (Findable, Accessible, Interoperable, and Reusable). This presentation examines the IPCC's experience over the past four years in curating and preserving digital objects, focusing on the implementation of FAIR and open data principles. We will explore the successes and setbacks of the AR6 experience, with particular attention to the development and application of a metadata schema. Finally, we will offer recommendations for consolidating and expanding this approach for AR7 to enhance transparency, reproducibility, and reusability of assessment outcomes.

This initiative aims to increase the transparency of IPCC's work, improve the reproducibility and reusability of assessment outcomes, optimize the utilization of the IPCC DDC's services, and promote compliance with open science best practices.

How to cite: Milward, D., Milward, A., and Xing, X.: Managing a FAIR Climate Change Data Catalogue: Lessons Learned from IPCC AR6 and Recommendations for AR7, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20454, https://doi.org/10.5194/egusphere-egu25-20454, 2025.

EGU25-20583 | Orals | ESSI3.2

International Earth, space, and environmental coordination of data and software management efforts 

Shelley Stall, Danie Kinkade, Natalie Raia, Lesley Wyborn, and Pedro Corrêa

The international Earth, space, environmental sciences informatics community has recently formed a new Research Data Alliance Community of Practice. Here we are focused on improving data and software management and sharing practices that result in our researchers having access to community informatics resources that support their research.  This community of practice will provide a place for teams and organizations in the Earth, space, and environmental research ecosystem to coordinate on common challenges, share information, review and consider RDA recommendations, seek leading practices, and work towards finding approaches to discipline-specific challenges and issues around data and software management and sharing. The international Earth, space, and environmental community is broad and includes researchers, data managers, data curators, institutions, instrument creators and manufacturers, software developers, tools, repositories, journal editors and more. 

An RDA community of practice is where those with common interests can collaborate on complex challenges that need multiple stakeholders to work through the layers of a solution. It is a place where projects can be highlighted and shared for the benefit of building collaboration and connection.     

Join us for this session and learn more about how we envision supporting the many global data and software management efforts.

How to cite: Stall, S., Kinkade, D., Raia, N., Wyborn, L., and Corrêa, P.: International Earth, space, and environmental coordination of data and software management efforts, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20583, https://doi.org/10.5194/egusphere-egu25-20583, 2025.

EGU25-21162 | Posters on site | ESSI3.2

Implementing FAIR Principles for Earth System Data: Insights from the European Eddy-Rich Earth-System Models (EERIE) project 

Heinrich Widmann, Chathurika Wickramage, and Fabian Wachsmann

We attempt to make EERIE data FAIR (Findable, Accessible, Interoperable, and Reusable) to enhance its scientific impact and utility. These principles of FAIRness ensure global access, integration, and reuse by researchers and decision-makers, thereby promoting collaboration and innovation.

Findability is enhanced through persistent identifiers such as DOIs and PIDs, ensuring data remains reliably locatable. Metadata standards, including CF conventions and CMIP standard names, ensure precise and efficient searchability. We enhance findability through data catalogs produced in the EERIE and nextGEMS projects, as well as platforms like World Data Center for Climate (WDCC) and DOKU. The WDCC ensures long-term storage with a focus on FAIRness, quality control, and DOI assignment following CF standards. Our EERIE data is also archived on DOKU with PIDs to ensure discoverability.

Accessibility is ensured by providing data through open protocols with clear terms of use. While accessibility does not always mean free access, it guarantees transparency and ease of use. Open-access repositories such as EERIE Cloud, Earth System Grid Federation (ESGF), and, WDCC combination with standardized formats such as NetCDF and Zarr, ensure broad accessibility. Additionally, tools like Zarr provide API access via HTTP, facilitating seamless and efficient data retrieval.

Interoperability is fundamental for integrating datasets across disciplines and platforms. The EERIE project supports this by linking datasets through initiatives such as EERIE Cloud, FREVA and by using standards such as CF conventions to ensure compatibility, facilitating multidisciplinary research.

Reusability is supported through detailed metadata, clear licensing models like CC-BY and CC0, and strong version control practices (e.g, v20240304). Documentation platforms such as easy.gems.dkrz.de assist users to understand and reproduce results. The maintenance of high data quality and the emphasis on archival and replication further enhance the long-term scientific use of these datasets.

Despite these efforts, the implementation of the FAIR data principles in a comprehensive manner poses significant challenges. In the EERIE project, for instance, we work with vast amounts of data, and standardizing it (e.g., CMORizing) can be complex. Obtaining CF-compliant names for all variables is particularly difficult, as there is often no one-to-one documentation from modeling groups. In some cases, this requires manually analyzing code to determine the correct definitions for certain variables.

For climate science, the application of FAIR principles is transformative. These efforts promote global collaboration, enhance the transparency of climate models, and equip policymakers with reliable data to address critical challenges such as climate adaptation and mitigation. Initiatives like EERIE cloud, ESGF and advancements in data processing, such as kerchunking massive datasets, further enhance the FAIRness of climate data, driving innovation and impact.

How to cite: Widmann, H., Wickramage, C., and Wachsmann, F.: Implementing FAIR Principles for Earth System Data: Insights from the European Eddy-Rich Earth-System Models (EERIE) project, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21162, https://doi.org/10.5194/egusphere-egu25-21162, 2025.

EGU25-21472 | Orals | ESSI3.2

Community Support and Engagement for FAIR Science in Climate Change Adaptation 

Erik Schultes and Barbara Magagna

Global climate change requires urgent and actionable adaptation planning.

Current Climate Change Adaptation (CCA) strategies often lack the necessary data and other relevant information to be scientifically competent. These limitations can complicate effective action and evaluation locally, and in combination with other regions. The recently awarded FAIR2Adapt Project aims to establish a comprehensive FAIR and open data framework for CCA and to demonstrate the impact of FAIR data on CCA strategies. By making CCA data FAIR, FAIR2Adapt will accelerate adaptation actions that are tailored to local needs.

Next to the technical development of FAIR data and services, a key issue in the effective uptake  of FAIR is the transfer of knowledge regarding FAIR practices, and in many cases hands-on skills related to the design, creation and governance of domain-relevant FAIR Enabling Resources.  Beginning in February 2025, the FAIR2Adapt, stakeholders (including members of it’s six use cases) will participate in FAIR awareness and training based on the GO FAIR Foundation’s FAIR Capacity Building Programme [https://zenodo.org/records/14187859]. This will include general FAIR Awareness workshops, training on the creation of FAIR Implementation Profiles and community-specific metadata and vocabulary in Metadata for Machine workshops. In addition to this, special attention will be given to the identification and prioritization of user requirements (both the technical approach in FAIR2Adapt as well as the case studies). Having both the technical expertise and building up the salient knowledge and skills, the FAIR2Adapt community will be well positioned to co-design, implement and share CCA related data and services that can accelerate meaningful and customized CCA. In this presentation, we will report the first draft user requirements for FAIR2Adapt and the emerging list of CCA community-specific FAIR Enabling Resources.  

 

How to cite: Schultes, E. and Magagna, B.: Community Support and Engagement for FAIR Science in Climate Change Adaptation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21472, https://doi.org/10.5194/egusphere-egu25-21472, 2025.

EGU25-21516 | Orals | ESSI3.2

Advancing Data Infrastructure for Chemical Risk Assessment and Exposome Research: The GENASIS Platform in the Context of FAIR Principles 

Katarína Řiháčková, Jana Borůvková, Zdenka Bednářová, Richard Hůlek, and Jana Klánová

Excellence in exposome research and chemical risk assessment (CRA) relies on robust capacities, innovative technologies, and skilled human resources. Research infrastructures are vital in providing access to these resources and driving innovation. Over recent decades, Europe has developed numerous research infrastructures, including EIRENE RI (Research Infrastructure for Environmental Exposure Assessment in Europe), the first EU research infrastructure dedicated to the human exposome. EIRENE RI aims to integrate interdisciplinary data, offering harmonized workflows and services to users across various sectors. Other initiatives, such as the Partnership for the Assessment of Risks from Chemicals (PARC), work on advancing harmonization and innovation in CRA.

A robust data infrastructure aligned with FAIR data and Open Science principles is essential for these research infrastructures. Mapping and evaluating the current data landscape is a critical step toward enhancing FAIR implementation and machine actionability. This contribution highlights existing strategies for harmonizing and managing global data on chemical occurrences developed through two decades, using the use case of the GENASIS information system.

GENASIS information is a platform originally developed for storing, harmonizing, and visualizing global environmental monitoring data. Over time, it has expanded to include data on chemical occurrences in indoor environments, consumer products, and human matrices. Today, it hosts over 3 million harmonized records on more than 800 chemicals, described with rich metadata, and it is continuously expanding. This enables the identification of gaps, locality comparisons, and evaluation of global trends in chemical concentrations in the environemnt and humans. GENASIS also serves as a model and sister database for the Global Monitoring Plan Data Warehouse of the Stockholm Convention and supports the United Nations Environment Programme in managing environmental and human monitoring data to evaluate the effectiveness of global treaties on chemical pollutants. GENASIS’ ongoing development and associated services contribute to the European Open Science Cloud (EOSC) in the Czech Republic, EIRENE RI and PARC initiatives.

This contribution evaluates GENASIS in terms of FAIR principles, detailing its current status, roadmap for further FAIR implementation, efforts to enhance machine actionability, and challenges encountered. The discussion is framed within the broader context of initiatives such as PARC, EIRENE RI, and EOSC CZ, emphasizing their role in advancing exposome research and CRA in Europe.

Acknowledgement: This project was supported from the European Union’s Horizon 2020 research and innovation programme under grant agreement No 857560 (CETOCOEN Excellence), and from the Horizon Europe programme under grant agreements No 101057014 (PARC) and 101079789 (EIRENE PPP). Views and opinions expressed are however those of the author(s) only and do not necessarily reflect those of the European Union, European Health and Digital Executive Agency (HADEA) or European Research Executive Agency (REA). Neither the European Union nor the granting authorities can be held responsible for any use that may be made of the information it contains. Authors thank the RECETOX Research Infrastructure (No LM2023069) financed by the Ministry of Education, Youth and Sports.

How to cite: Řiháčková, K., Borůvková, J., Bednářová, Z., Hůlek, R., and Klánová, J.: Advancing Data Infrastructure for Chemical Risk Assessment and Exposome Research: The GENASIS Platform in the Context of FAIR Principles, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21516, https://doi.org/10.5194/egusphere-egu25-21516, 2025.

EGU25-21605 | Orals | ESSI3.2

Status, issues and challenges with FAIRness of seismological waveform data and beyond 

Florian Haslinger, Lesley Wyborn, Rob Casey, Helle Pederson, Elisabetta D’Anastasio, Javier Quinteros, Jonathan Hanson, and Jerry Carter

Driven by the scientific need for global exchange of data to study earthquakes and related phenomena, community standards and best practices have evolved in seismology for decades. These developments are largely driven by operational and scientific requirements coming directly from the community of academic research and seismological monitoring, and have resulted in standardised data formats, data models and services for data access and exchange.

Initial developments, promotion and further evolution of these standards are coordinated mainly within the International Federation of Digital Seismic Networks (FDSN, https://fdsn.org), a commission of IASPEI (International Association of Seismology and Physics of the Earth's Interior, httwww.iaspei.org) that is one of eight associations of the IUGG (International Union of Geodesy and Geophysics, https://iugg.org).   

With the introduction of the FAIR (Findable, Accessible, Interoperable, Reusable) principles in 2016 and the subsequent appearance of FAIR assessment methods and tools it became clear that these seismological community standards only cover parts of the FAIR principles. Interoperability remains challenging, for example, due to the lack of community standardised FAIR vocabularies, and the lack of a harmonised and consistently applied data license policy impacts Reproducibility.

The emergence of new data types and the drastic increase in data volumes due to new measurement techniques require updates and evolution of the existing community standards, highlighting another general challenge:  Who are the recognised and appropriate governance bodies for curation and further development of 'relevant community standards' (as required by the FAIR principles)?

In this presentation we describe the current status of FAIRness for seismological waveform data and beyond, also looking towards seismology in general, geodesy and some other fields of geophysics. Based on our assessment of current challenges we discuss open questions and possible ways forward. We look at FAIR-relevant development and governance of standards, the potential role of existing international organisations like FDSN, IASPEI and IUGG, and the possibility and need to coordinate across domains for harmonisation as well as demarcation.   

How to cite: Haslinger, F., Wyborn, L., Casey, R., Pederson, H., D’Anastasio, E., Quinteros, J., Hanson, J., and Carter, J.: Status, issues and challenges with FAIRness of seismological waveform data and beyond, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21605, https://doi.org/10.5194/egusphere-egu25-21605, 2025.

EGU25-1511 | ECS | Orals | ESSI3.3

A workflow for cloud-based and HPC simulations with the NEMO ocean model using containers 

Aina Gaya-Àvila, Bruno de Paula Kinoshita, Stella V. Paronuzzi Ticco, Oriol Tintó Prims, and Miguel Castrillo

In this work, we explored the deployment and execution of the NEMO ocean model using Singularity containers within the EDITO Model Lab, implementing the European Digital Twin of the Ocean. The Auto-NEMO workflow, a fork of Auto-EC-Earth used to run NEMO workflows using the NEMO Community reference code, was adapted to run simulations using containers. The use of a Singularity container ensures consistent execution by packaging all dependencies, making it easier to deploy the model across various HPC systems.

The containerized approach was tested on multiple HPC platforms, including MareNostrum5 and LUMI, to evaluate scaling performance. Our tests compared the use of mpich and openmp libraries, providing insights into how communication strategies impact the computational performance of the model in containerized setups. In addition, the runs are orchestrated by a content workflow manager, in this case Autosubmit, deployed in a cloud infrastructure in EDITO-Infra, making the entire solution (workflow manager and workflow itself) portable end-to-end. The benefits of portability and reproducibility make containers an attractive solution for streamlining workflows in diverse computational environments.

A comparison between containerized and non-containerized runs highlights the trade-offs involved. Direct execution may provide slightly better performance in some cases, but the containerized approach greatly reduces setup complexity. These findings demonstrate the potential of containerization to enhance efficiency and accessibility in large-scale ocean modeling efforts.

How to cite: Gaya-Àvila, A., de Paula Kinoshita, B., Paronuzzi Ticco, S. V., Tintó Prims, O., and Castrillo, M.: A workflow for cloud-based and HPC simulations with the NEMO ocean model using containers, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1511, https://doi.org/10.5194/egusphere-egu25-1511, 2025.

EGU25-2142 | ECS | Posters on site | ESSI3.3

Enhancing Data Provenance in Workflow Management: Integrating FAIR Principles into Autosubmit and SUNSET 

Albert Puiggros, Miguel Castrillo, Bruno de Paula Kinoshita, Pierre-Antoine Bretonniere, and Victòria Agudetse

Ensuring robust data provenance is paramount for advancing transparency, traceability, and reproducibility in climate research. This work presents the integration of FAIR (Findable, Accessible, Interoperable, and Reusable) principles into the workflow management ecosystem through provenance integration in Autosubmit, a workflow manager developed at the Barcelona Supercomputing Center (BSC), and SUNSET (SUbseasoNal to decadal climate forecast post-processing and asSEmenT suite), an R-based verification workflow also developed at the BSC.

Autosubmit supports the generation of data provenance information based on RO-Crate, facilitating the creation of machine-actionable digital objects that encapsulate detailed metadata about its executions. Autosubmit integrates persistent identifiers (PIDs) and schema.org annotations, making provenance records more accessible and actionable for both humans and machines.  However, the provenance metadata provided by Autosubmit through RO-Crate focuses on the workflow process and does not encapsulate the details of the data transformation processes. This is where SUNSET plays a complementary role. SUNSET’s approach for provenance information is based on the METACLIP (METAdata for CLImate Products) ontologies. METACLIP offers a semantic approach for describing climate products and their provenance. This framework enables SUNSET to provide specific, high-resolution  provenance metadata for its operations, improving transparency and compliance with FAIR principles. The generated files provide detailed information about each transformation the data has undergone, as well as additional details about the data's state, location, structure, and associated source code, all represented in a tree-like structure.

The main contribution of this work is the generation of a comprehensive provenance object by integrating these tools. SUNSET uses Autosubmit to parallelize its data processing tasks, with Autosubmit managing SUNSET jobs. As part of this process, an RO-Crate is automatically generated describing the overall execution. This object encapsulates detailed provenance metadata for each individual job within the workflow, using METACLIP's semantic framework to represent each SUNSET execution process. Certain schema.org entities are introduced to have the RO-Crate created by Autosubmit link with the provenance details generated by SUNSET. This integrated approach provides a unified hierarchical provenance record that spans to both the workflow management system and the individual job executions, ensuring that provenance objects are automatically generated for each experiment conducted.

This work demonstrates the practical application of FAIR principles in climate research by advancing provenance tracking within complex workflows. It represents an initial step to obtain and share metadata about the provenance of the data products that a workflow provides. The integration of RO-Crate and METACLIP not only enhances the reproducibility of climate data products but also fosters greater confidence in their reliability. To our knowledge, this is the first effort in the climate domain to combine different provenance formats into a single object, aiming to obtain a complete provenance graph with all the metadata. 

How to cite: Puiggros, A., Castrillo, M., de Paula Kinoshita, B., Bretonniere, P.-A., and Agudetse, V.: Enhancing Data Provenance in Workflow Management: Integrating FAIR Principles into Autosubmit and SUNSET, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2142, https://doi.org/10.5194/egusphere-egu25-2142, 2025.

EGU25-4355 | ECS | Posters on site | ESSI3.3

Generic State Vector: streaming and accessing high resolution climate data from models to end users 

Iker Gonzalez-Yeregi, Pierre-Antoine Bretonnière, Aina Gaya-Avila, and Francesc Roura-Adserias

The Climate Adaptation Digital Twin (ClimateDT) is a contract under the Destination Earth initiative (DestinE) that aims to develop a digital twin to account for climate change adaptation. This is achieved by running high-resolution simulations with different climate models by making use of the different EuroHPC platforms. In addition to the climate models, applications that consume data from models are also developed under the contract. A common workflow is used to execute the whole pipeline from the model launching to the data consumption by the applications in a user-friendly and automated way.

One of the challenges of this complex workflow is to handle the different outputs that each of the climate models initially offered. Each model works with its own grid, vertical levels, and variable set. These differences in format make it very complicated for applications to consume and compare data coming from different models in an automated and timely manner. This issue is resolved by introducing the concept of Generic State Vector (GSV), which defines a common output portfolio for all models to ensure a homogeneous output between models. The conversion from the model's native output to the GSV happens before the data is written in the HPC and it is automated in the workflow allowing transparent access to the data changing only the name of the model in the call.

Data in the GSV format can be read using a newly designed dedicated Python tool: the GSV Interface. This tool links the model part of the workflow with the applications part of the workflow, enabling running everything in a single complex workflow (end-to-end workflow). The GSV Interface allows to read data that has been previously converted to GSV, adding proper metadata. It also offers some extra features like interpolation to regular grids and area selection. All the workflow components that read data from the models rely on the GSV Interface. In addition to that, the GSV Interface can also be used to transparently retrieve and process data from the public Destination Earth Service Platform.

How to cite: Gonzalez-Yeregi, I., Bretonnière, P.-A., Gaya-Avila, A., and Roura-Adserias, F.: Generic State Vector: streaming and accessing high resolution climate data from models to end users, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4355, https://doi.org/10.5194/egusphere-egu25-4355, 2025.

EGU25-4466 | ECS | Posters on site | ESSI3.3

ClimateDT Workflow: A containerized climate workflow 

Francesc Roura-Adserias, Aina Gaya-Avila, Leo Arriola i Meikle, Iker Gonzalez-Yeregi, Bruno De Paula Kinoshita, Jaan Tollander de Balsch, and Miguel Castrillo

The Climate Adaptation Digital Twin (ClimateDT), a contract (DE_340) inside the Destination Earth (DestinE) flagship initiative from the European Commission, is a highly collaborative project where climate models are executed in an operational manner on different EuroHPC platforms. The workflow software supporting such executions, called ClimateDT Workflow, contains a model component and an applications component. The applications can be seen as elements that consume the data that is provided by the climate models. They aim to provide climate information to sectors that are critically dependent on climate change, such as renewable energy or wildfires, among others. This workflow relies on the Autosubmit workflow manager and is executed over different EuroHPC platforms that are part of the contract.

There are six lightweight applications that are run in this workflow, in parallel to the model and in a streaming fashion. Setting up and maintaining an environment for these applications for each EuroHPC platform (plus the development environments) is a time-consuming and cumbersome task. These machines are shared by multiple users, have different operating systems and libraries, some do not have internet access for all users on their login nodes, and there are different rules to install and maintain software on each machine.

In order to overcome these difficulties all the application-required dependencies of the workflow are encapsulated beforehand in a Singularity container and therefore the portability to the different platforms becomes merely an issue with path-binding inside the platform. Through the use of Singularity containers, their execution does not require administrator permissions, which allows anyone with access to the project to execute the desired application either on the EuroHPC machines, or on their local development environment.

This work shows the structure of the ClimateDT workflow and how it uses Singularity containers, how they contribute not only to portability but also to traceability and provenance, and finally the benefits and issues found during its implementation. We believe that the successful use of containers in this climate workflow, where applications run in parallel to the climate models in a streaming fashion and where the complete workflow runs on different HPC platforms, presents a good reference for other projects and workflows that must be platform-agnostic and that require agile portability of their components.

How to cite: Roura-Adserias, F., Gaya-Avila, A., Arriola i Meikle, L., Gonzalez-Yeregi, I., De Paula Kinoshita, B., Tollander de Balsch, J., and Castrillo, M.: ClimateDT Workflow: A containerized climate workflow, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4466, https://doi.org/10.5194/egusphere-egu25-4466, 2025.

In an era of unprecedented availability of Earth Observation (EO) data, the Copernicus Data Space Ecosystem (CDSE) emerges as a vital platform to bridge the gap between data accessibility and actionable insights. With petabytes of freely accessible satellite data at our fingertips and multiple operational data processing platforms in place, many of the foundational challenges of accessing and processing sensor data have been addressed. Yet, the widespread adoption of EO-based applications remains below expectations. The challenge lies in the effective extraction of relevant information from the data. While numerous R&D projects demonstrate the possibilities of EO, their results are often neither repeatable nor reusable, primarily due to prototype-level implementations and overly tailored, non-standardized workflows.  

CDSE tackles these barriers by adopting common standards and patterns, most notably through openEO, an interface designed to standardize EO workflow execution across platforms. openEO enables the development of reusable workflows that are scalable and transferable, paving the way for systematic and objective monitoring of the planet. CDSE has already integrated openEO as a core processing interface, and further advancements are underway, including the integration of Sentinel Hub to support openEO. This integration will enhance instantaneous visualization, synchronous API requests, and batch processing, as well as support openEO process graphs within the Copernicus Browser, bringing the simplicity and speed of Sentinel Hub’s synchronous engine to the openEO ecosystem.  

CDSE’s openEO capabilities are already validated through large-scale operational projects such as ESA WorldCereal and Copernicus Global Land Cover and Tropical Forestry Mapping and Monitoring Service (LCFM), which leverage its robust, scalable, and reliable infrastructure. Additionally, the openEO Algorithm Plaza fosters collaboration by enabling the easy sharing and reuse of processing workflows, while the Bring Your Own Data feature allows users to integrate their datasets into the ecosystem, promoting data interoperability and collaborative advancements.  

CDSE is embracing a federated approach, allowing additional data or service providers to become part of the ecosystem. This inclusivity ensures a growing network of interoperable services while maintaining technical and operational stability—a cornerstone for broad adoption and long-term sustainability.  

By addressing the need for operational and reusable workflows with openEO and related initiatives, CDSE is not only advancing the technical landscape of EO but also fostering a culture of repeatable, scalable, and impactful science. Through this session, we aim to spark a discussion on how to make EO applications more accessible, reusable, and impactful for the global community.

How to cite: Sharma, P.: How openEO standardizes workflows for scalable and reusable EO data analysis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5593, https://doi.org/10.5194/egusphere-egu25-5593, 2025.

EGU25-6201 | Orals | ESSI3.3

Advancing Computational Workflow Sharing in Earth Science: Insights from DT-GEO and Geo-INQUIRE 

Marco Salvi, Rossana Paciello, Valerio Vinciarelli, Kety Giuliacci, Daniele Bailo, Pablo Orviz, Keith Jeffery, Manuela Volpe, Roberto Tonini, and Alejandra Guerrero

The increasing complexity and volume of data in Solid Earth Science necessitate robust solutions for workflow representation, sharing, and reproducibility. Within the DT-GEO (https://dtgeo.eu/) project, we addressed the challenge of creating interoperable and discoverable representations of computational workflows to facilitate data reuse and collaboration. Leveraging the EPOS Platform (https://www.epos-eu.org/), a multidisciplinary research infrastructure focused on Solid Earth Science, we aimed to expose workflows, datasets, and software to the community while adhering to the FAIR (Findable, Accessible, Interoperable, and Reusable) principles. While the EPOS-DCAT-AP (https://github.com/epos-eu/EPOS-DCAT-AP) model, already used in EPOS, can effectively represent datasets and software, it lacks direct support for computational workflows, necessitating the adoption of alternative standards.

To overcome this limitation, we employed the Common Workflow Language (CWL, https://www.commonwl.org/) to describe workflows, capturing their structure, software, datasets, and dependencies. The developed CWL representations are "abstract" focusing on general workflow structures while omitting execution-specific details to prioritize interoperability. To package these workflows along with metadata, we utilized Workflow Run Crate, an extension of the RO-Crate (https://www.researchobject.org/ro-crate/) standard. Together, these technologies enable workflows to become self-contained entities, simplifying sharing and reuse. 

This approach not only aligns with community standards but also benefits from a mature ecosystem of tools and libraries, ensuring seamless integration and widespread applicability. Initial implementations within the DT-GEO project serve as a model for adoption in related initiatives such as Geo-INQUIRE (https://www.geo-inquire.eu/), where similar methodologies are being used to share workflows derived from the Simulation Data Lake (SDL) infrastructure. These implementations pave the way for broader integration within the EPOS Platform, enhancing access to advanced workflows across disciplines.

Our contribution highlights the value of adopting standardized tools and methodologies for workflow management in Solid Earth Science, showcasing how CWL and RO-Crate streamline interoperability and foster collaboration. These advances address challenges in data and computational management, contributing to the scalable FAIR workflows essential for tackling the complexities of Solid Earth Science. Moving forward, the integration of these standards across projects like DT-GEO and Geo-INQUIRE will further enhance the EPOS Platform's capabilities, offering a unified gateway to reproducible, secure, and trustworthy workflows that meet the evolving needs of the scientific community.

How to cite: Salvi, M., Paciello, R., Vinciarelli, V., Giuliacci, K., Bailo, D., Orviz, P., Jeffery, K., Volpe, M., Tonini, R., and Guerrero, A.: Advancing Computational Workflow Sharing in Earth Science: Insights from DT-GEO and Geo-INQUIRE, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6201, https://doi.org/10.5194/egusphere-egu25-6201, 2025.

EGU25-6216 | Posters on site | ESSI3.3

CAMELS-PLUS: Enhancing Hydrological Data Through FAIR Innovations. 

Carlos Zuleta Salmon, Mirko Mälicke, and Alexander Dölich

The CAMELS-PLUS initiative is revolutionizing the way hydrological, and Earth System Science (ESS) data are processed, shared, and utilized by enhancing the widely-used CAMELS-DE dataset. While Germany boasts one of the richest hydrological datasets globally, CAMELS-DE has faced challenges due to its reliance on fragmented, manual workflows, which are error-prone and hinder collaboration. CAMELS-PLUS introduces a groundbreaking solution: a standardized framework for containerized scientific tools that embed rich metadata, ensuring provenance, reusability, and seamless integration across diverse scientific domains.

A key innovation of CAMELS-PLUS lies in its ability to bridge the gap between disciplines by implementing a fully containerized pipeline for dataset pre-processing. This approach allows researchers in meteorology, forestry, and other ESS subdomains to easily contribute and extend CAMELS-DE without the complexity of navigating storage systems or inconsistent workflows. The initiative’s metadata schema, implemented as YAML files with JSON-based tool parameterization, enables tools to "speak the same language," ensuring they are interoperable and aligned with FAIR principles.

Key Deliverables:

  • Updated CAMELS-DE Dataset: Incorporates new precipitation sources and enhanced metadata for seamless integration with the NFDI4Earth Knowledge Hub.
  • Standardized Scientific Containers: A community-adopted specification for containerized tools, promoting accessibility and reusability across disciplines.
  • Interactive Community Engagement: Extensions to camels-de.org, transforming it into a hub for exploring workflows and fostering interdisciplinary collaboration.

What makes CAMELS-PLUS particularly compelling is its potential to democratize access to cutting-edge hydrological datasets. By enabling non-specialists to contribute and utilize CAMELS-DE through intuitive, containerized workflows, the initiative reduces barriers to entry and accelerates innovation in data-driven hydrology and beyond. This project not only sets a new standard for dataset management in ESS but also creates a replicable model for tackling similar challenges across other scientific domains. CAMELS-PLUS is poised to inspire transformative changes in how large-sample datasets are curated, shared, and advanced for global scientific impact.

How to cite: Zuleta Salmon, C., Mälicke, M., and Dölich, A.: CAMELS-PLUS: Enhancing Hydrological Data Through FAIR Innovations., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6216, https://doi.org/10.5194/egusphere-egu25-6216, 2025.

EGU25-6544 | Posters on site | ESSI3.3

PyActiveStorage:  Efficient distributed data analysis using Active Storage for HDF5/NetCDF4 

Bryan N. Lawrence, David Hassell, Grenville Lister, Predoi Valeriu, Scott Davidson, Mark Goddard, Matt Pryor, Stig Telfer, Konstantinos Chasapis, and Jean-Thomas Acquaviva

Active storage (also known as computational storage) has been a concept often proposed but not often delivered. The idea is that there is a lot of under-utilised compute power in modern storage systems, and this could be utilised to carry out some parts of data analysis workflows. Such a facillity would reduce the cost of moving data, and make distributed data analysis much more efficient.

For storage to be able to handle compute, either an entire compute stack has to be migrated to the storage (with all the problems around security and dependencies) or the storage has to offer suitable compute interfaces. Here we take the second approach, borrowing the concept of providing system reduction operations in the MPI interface of HPC systems, to define and implement a reduction interface for the complex layout of HDF5 (and NetCDF4) data.

We demonstrate a near-production quality deployment of the technology (PyActiveStorage) fronting JASMIN object storage, and describe how we have built a POSIX prototype. The first provides compute “near” the storage, the second is truly “in” the storage. The performance with the object store is such that for some tasks distributed workflows based on reduction operations on HDF5 data can be competitive with local workflow speeds, a result which has significant implications for avoiding expensive copies of data and unnecessary data movement. As a byproduct of this work, we have also upgraded a pre-existing pure python HDF5 reader to support lazy access, which opens up threadsafe read operations on suitable HDF5 and NetCDF4 data.

To our knowledge, there has previously been no previous practical demonstration of active storage for scientific data held in HDF5 files. While we have developed this technology with application in distributed weather and climate workflows, we believe it will find utility in a wide range of scientific workflows.

How to cite: Lawrence, B. N., Hassell, D., Lister, G., Valeriu, P., Davidson, S., Goddard, M., Pryor, M., Telfer, S., Chasapis, K., and Acquaviva, J.-T.: PyActiveStorage:  Efficient distributed data analysis using Active Storage for HDF5/NetCDF4, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6544, https://doi.org/10.5194/egusphere-egu25-6544, 2025.

EGU25-7056 | Orals | ESSI3.3

Reliable and reproducible Earth System Model data analysis with ESMValTool 

Valeriu Predoi and Bouwe Andela

ESMValTool is a software tool for analyzing data produced by Earth System Models (ESMs) in a reliable and reproducible way. It provides a large and diverse collection of “recipes” that reproduce standard, as well as state-of-the-art analyses. ESMValTool can be used for tasks ranging from monitoring continuously running ESM simulations to analysis for scientific publications such as the IPCC reports, including reproducing results from previously published scientific articles as well as allowing scientists to produce new analysis results. To make ESMValTool a user-friendly community tool suitable for doing open science, it adheres to the FAIR principles for research software. It is: - Findable - it is published in community registries, such as https://research-software-directory.org/software/esmvaltool; - Accessible - it can be installed from Python package community distribution channels such as conda-forge, and the open-source code is available on Zenodo with a DOI, and on GitHub; - Interoperable - it is based on standards: it works with data that follows CF Conventions and the Coupled Model Intercomparison Project (CMIP) Data Request, its reusable recipes are written in YAML, and provenance is recorded in the W3C PROV format. It supports diagnostics written in a number of programming language, with Python and R being best supported. Its source code follows the standards and best practices for the respective programming languages; - Reusable - it provides a well documented recipe format and Python API that allow reusing previous analyses and building new analysis with previously developed components. Also, the software can be installed from conda-forge and DockerHub and can be tailored by installing from source from GitHub. In terms of input data, ESMValTool integrates well with the Earth System Grid Federation (ESGF) infrastructure. It can find, download and access data from across the federation, and has access to large pools of observational datasets. ESMValTool is built around two key scientific software metrics: scalability and user friendliness. An important aspect of user friendliness is reliability. ESMValTool is built on top of the Dask library to allow scalable and distributed computing, ESMValTool also uses parallelism at a higher level in the stack, so that jobs can be distributed on any standard High Performance Computing (HPC) facility; and software reliability and reproducibility - our main strategy to ensure reliability is modular, integrated, and tested design. This comes back at various levels of the tool. We try to separate commonly used functionality from “one off” code, and make sure that commonly used functionality is covered by unit and integration tests, while we rely on regression testing for everything else. We also use comprehensive end-to-end testing for all our “recipes” before we release new versions. Our testing infrastructure ranges from basic unit tests to tools that smartly handle various file formats, and use image comparison algorithms to compare figures. This greatly reduces the need for ‘human testing’, allowing for built-in robustness through modularity, and a testing strategy that has been tailored to match the technical skills of its contributors.

How to cite: Predoi, V. and Andela, B.: Reliable and reproducible Earth System Model data analysis with ESMValTool, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7056, https://doi.org/10.5194/egusphere-egu25-7056, 2025.

EGU25-7070 | Posters on site | ESSI3.3

EarthCODE - a FAIR and Open Environment for collaborative research in Earth System Science  

Chandra Taposeea-Fisher, Garin Smith, Ewelina Dobrowolska, Daniele Giomo, Francesco Barchetta, Stephan Meißl, and Dean Summers

The Open Science and Innovation Vision included in ESA’s EO Science Strategy (2024) addresses 8 key elements: 1) openness of research data, 2) open-source scientific code, 3) open access papers with data and code; 4) standards-based publication and discovery of scientific experiments, 5) scientific workflows reproducible on various infrastructures, 6) access to education on open science, 7) community practice of open science; and 8) EO business models built on open-source. EarthCODE (https://earthcode.esa.int) is a strategic ESA EO initiative to support the implementation of this vision. 

EarthCODE (Earth Science Collaborative Open Development Environment) will form part of the next generation of cloud-based geospatial services, aiming towards an integrated, cloud-based, user-centric development environment for European Space Agency’s (ESA) Earth science activities. EarthCODE looks to maximise long-term visibility, reuse and reproducibility of the research outputs of such projects, by leveraging FAIR and open science principles and enabling, thus fostering a sustainable scientific process. EarthCODE proposes a flexible and scalable architecture developed with interoperable open-source blocks, with a long-term vision evolving by incrementally integrating industrially provided services from a portfolio of the Network of Resources.  Additionally, EarthCODE is a utilisation domain of EOEPCA+, contributing to the development and evolution of Open Standards and protocols, enabling internationally interoperable solutions.  

EarthCODE will provide an Integrated Development Platform, giving developers tools needed to develop high quality workflows, allowing experiments to be executed in the cloud and be end-to-end reproduced by other scientists. EarthCODE is built around existing open-source solutions, building blocks and platforms, such as the Open Science Catalogue, EOxHub and EOEPCA. It has additionally begun to integrate platform services from DeepESDL, Euro Data Cube, Polar TEP and the openEO federation on CDSE platforms, with more being added annually through ESA best practices. With it’s adopted federated approach, EarthCODE will facilitate processing on other platforms, i.e. DeepESDL, ESA EURO Data Cube, Open EO Cloud/Open EO Platform and AIOPEN/AI4DTE.   

The roadmap for the portal includes the initial portal release by end of 2024, followed by the capability to publish experiments in Q1 2025 (including development, publishing, finding and related community engagement), and by mid-2025 to have a further release with reproducibility capabilities around accessibility and execute functionalities.  

Collaboration and Federation are at the heart of EarthCODE. As EarthCODE evolves we expect providing solutions allowing federation of data and processing. EarthCODE has ambition to deliver a model for a Collaborative Open Development Environment for Earth system science, where researchers can leverage the power of the wide range of EO platform services available to conduct their science, while also making use of FAIR Open Science tools to manage data, code and documentation, create end-to-end reproducible workflows on platforms, and have the opportunity to discover, use, reuse, modify and build upon the research of others in a fair and safe way. Overall, EarthCODE aims to enable elements for EO Open Science and Innovation vision, including open data, open-source code, linked data/code, open-access documentation, end-to-end reproducible workflows, open-science resources, open-science tools, and a healthy community applying all the elements in their practice.

How to cite: Taposeea-Fisher, C., Smith, G., Dobrowolska, E., Giomo, D., Barchetta, F., Meißl, S., and Summers, D.: EarthCODE - a FAIR and Open Environment for collaborative research in Earth System Science , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7070, https://doi.org/10.5194/egusphere-egu25-7070, 2025.

EGU25-8114 | ECS | Orals | ESSI3.3

Flexible and scalable workflow framework HydroFlows for compound flood risk assessment and adaptation modelling 

Willem Tromp, Dirk Eilander, Hessel Winsemius, Tjalling De Jong, Brendan Dalmijn, Hans Gehrels, and Bjorn Backeberg

Flood risk assessments are increasingly guiding urban developments to safeguard against flooding. These assessments, consisting mainly of hazard and risk maps, make use of interconnected models consisting of a chain of climate, hydrological, hydraulic, and impact models, which are increasingly run interactively to support scenario modelling and decision-making in digital twins. To maintain interoperability, transparency, and reusability of this chain and the assessments themselves, using a workflow manager to manage the inter-model dependencies is a natural fit. However, composing and maintaining workflows is a non-trivial, time-consuming task, and they often have to be refactored for new workflow engines, or when changing compute environments, even if the workflow conceptually remains unchanged. These issues are particularly relevant in the development of digital twins for climate adaptation, where flood risk assessments serve as input to indicate high-risk areas. The complex model chain underpinning such digital twins can benefit greatly from transparent workflows that can be easily reused across different contexts.

To address these challenges, we developed the HydroFlows Python framework for composing and maintaining flood risk assessment workflows by leveraging common patterns identified across different workflows. The framework allows users to use one of the many steps available in the library or define workflow steps themselves and combine these into complete workflows which are validated on the fly. Available workflow steps include building, running, and postprocessing of models. Execution of the workflow is handled by one of the workflow managers to which our workflow description can be exported, such as Snakemake or tools with CWL support. This flexibility allows users to easily scale their workflows to different compute environments whenever the computational requirements demand so.

We demonstrate the flexibility of the HydroFlows framework by highlighting how it can be used to create complex workflows needed for digital twins supporting climate adaptation. HydroFlows not only enhances the flexibility and portability of the digital twin modelling workflows but also facilitates the integration of digital twin tooling and advanced computing and processing solutions to support interactive flood risk assessments in federated compute and data environments.

How to cite: Tromp, W., Eilander, D., Winsemius, H., De Jong, T., Dalmijn, B., Gehrels, H., and Backeberg, B.: Flexible and scalable workflow framework HydroFlows for compound flood risk assessment and adaptation modelling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8114, https://doi.org/10.5194/egusphere-egu25-8114, 2025.

EGU25-8305 | ECS | Posters on site | ESSI3.3

Enabling reliable workflow development with an advanced Testing Suite 

Alejandro Garcia Lopez, Leo Arriola Meikle, Gilbert Montane Pinto, Miguel Castrillo, Bruno de Paula Kinoshita, Eric Ferrer Escuin, and Aina Gaya Avila

Climate simulations require complex workflows that often integrate multiple components and different configurations per experiment, typically involving high-performance computing resources. The exhaustive testing required for these workflows can be time and resource consuming, presenting significant challenges in terms of computational cost and human effort. However, robust Continuous Integration (CI) testing ensures the reliability and reproducibility of such complex workflows by validating the codebase and ensuring the integrity of all the components used when performing climate simulations. Additionally, CI testing facilitates both major and minor releases, enhancing the efficiency of the development lifecycle.

To address these challenges, we present our Testing Suite software, designed to automate the setup, configuration, and execution of integration tests using Autosubmit, a workflow manager developed at the BSC. Autosubmit is typically used for climate modelling experiments, but also atmospheric composition ones, and also constitutes the backbone of some operational systems and Digital Twin initiatives. The Testing Suite software allows Autosubmit commands to be executed in batches and the responses from the Workflow Manager to be bypassed in a structured manner. By streamlining this process, it minimizes the effort required for exhaustive testing while ensuring reliability.

Beyond integration testing, the Testing Suite offers advanced capabilities for scientific result verification. By automatically comparing output data bit by bit, it swiftly detects regressions during test execution. Additionally, it provides CPMIP performance metrics, offering insights into the efficiency of the workflows.

As a result, the Testing Suite plays an important role in quality assurance, particularly during releases, where extensive testing ensures the workflow meets required functionality and performance standards across different configurations. These integration tests act as a checkpoint, validating the stability and robustness of the software before release. They also identify stable points in the main codebase, enabling developers to create new branches with confidence. This approach minimizes compatibility issues and facilitates a smoother development process.

In conclusion, the Testing Suite is a crucial part of the development lifecycle for climate simulations. It mitigates risks, ensures stability, and fosters innovation, all while maintaining a robust and reliable foundation for scientific research and development.

How to cite: Garcia Lopez, A., Arriola Meikle, L., Montane Pinto, G., Castrillo, M., de Paula Kinoshita, B., Ferrer Escuin, E., and Gaya Avila, A.: Enabling reliable workflow development with an advanced Testing Suite, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8305, https://doi.org/10.5194/egusphere-egu25-8305, 2025.

EGU25-8621 | ECS | Posters on site | ESSI3.3

Auto-EC-Earth: An automatic workflow to manage climate modelling experiments using Autosubmit 

Eric Ferrer, Gilbert Montane, Miguel Castrillo, and Alejandro Garcia

The European community Earth system model EC-Earth is based on different and interoperable climate components simulating different processes of the Earth system. This makes it a complex model that requires multiple input data sources for its various model components, which can be run in parallel with multiple configurations and resolutions, demanding different computational resources in each case.

The EC-Earth software contains a minimum set of scripts to manage the compilation and execution of the simulations, but these are not enough to perform all the tasks that experiments demand nor to guarantee the traceability and reproducibility of the entire workflow in a high-productivity scientific environment. For that matter, the Auto-EC-Earth software has been developed at the Earth Sciences department of the Barcelona Supercomputing Center (BSC-ES) relying on Autosubmit, a workflow manager also developed at BSC-ES.

We take advantage of the automatization provided by the workflow manager that allows us to configure, manage, orchestrate and share experiments with different configurations and target platforms. The workflow manager allows the user to split the run into different tasks that are executed on different local and remote machines, like the HPC platform where the simulation needs to be performed. This is achieved in a seamless integration between Autosubmit, the EC-Earth tools, and the different machines where the scripts run, all without any user-input required after the initial setup and the launch of the experiment thanks to the workflow developments. Autosubmit also allows to ensure traceability of the actual runs, to have all the required data available for different kinds of experiments separated and well documented.

However, running the main part of the simulation is a cooperative task between the Autosubmit workflow manager and the different tools used for each model version. Auto-EC-Earth workflow has evolved to adapt the best possible to the EC-Earth model scripts that are present to help with the model runs. In EC-Earth 4, ScriptEngine is used to manage the run, and it has been fully integrated into the Auto-EC-Earth 4 workflow and used to set up the environment, while Autosubmit still manages the submission of jobs to the HPC and the dependencies between them.

Auto-EC-Earth is a great example of a workflow system that has been developed and used throughout the years, well established within the BSC-ES and used in multiple production cases, like multiple CMIP exercises as well as a reference for newer ESM workflows like the one developed in the Destination Earth project. It has also allowed the BSC-ES to collaborate with the EC-Earth community through the testing of the new releases of the model.

How to cite: Ferrer, E., Montane, G., Castrillo, M., and Garcia, A.: Auto-EC-Earth: An automatic workflow to manage climate modelling experiments using Autosubmit, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8621, https://doi.org/10.5194/egusphere-egu25-8621, 2025.

EGU25-9175 | Posters on site | ESSI3.3

Enhancing Earth system models efficiency: Leveraging the Automatic Performance Profiling tool 

Roc Salvador Andreazini, Xavier Yepes Arbós, Stella Valentina Paronuzzi Ticco, Oriol Tintó Prims, and Mario Acosta Cobos

Earth system models (ESMs) are essential to understand and predict climate variability and change. However, their complexity and computational demands of high-resolution simulations often lead to performance bottlenecks that can impede research progress. Identifying and resolving these inefficiencies typically require significant expertise and manual effort, posing challenges for both climate scientists and High Performance Computing (HPC) engineers.

We propose automating performance profiling as a solution to help researchers concentrate on improving and optimizing their models without the complexities of manual profiling. The Automatic Performance Profiling (APP) tool brings this solution to life by streamlining the generation of detailed performance reports for climate models.

The tool ranges from high-level performance metrics, such as Simulated Years Per Day (SYPD), to low-level metrics, such as PAPI counters and MPI communication statistics. This dual-level reporting makes the tool accessible to a wide range of users, from climate scientists seeking a general understanding of the model efficiency, to HPC experts requiring granular insights for advanced optimizations.

Seamlessly integrated with Autosubmit, the workflow manager developed at the Barcelona Supercomputing Center (BSC), APP ensures compatibility with complex climate modelling workflows. By automating the collection and reporting of key metrics, APP reduces the effort and expertise needed for performance profiling, empowering users to enhance the scalability and efficiency of their climate models.

APP currently supports multiple models, including the EC-Earth4 climate model and the NEMO ocean model, and is compatible with different HPC systems, such as Marenostrum 5 and ECMWF’s supercomputer. Furthermore, the modular design of the tool allows adding new models and HPC platforms easily.

How to cite: Salvador Andreazini, R., Yepes Arbós, X., Paronuzzi Ticco, S. V., Tintó Prims, O., and Acosta Cobos, M.: Enhancing Earth system models efficiency: Leveraging the Automatic Performance Profiling tool, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9175, https://doi.org/10.5194/egusphere-egu25-9175, 2025.

Geo-simulation experiments (GSEs) are experiments allowing the simulation and exploration of Earth’s surface (such as hydrological, geomorphological, atmospheric, biological, and social processes and their interactions) with the usage of geo-analysis models (hereafter called ‘models’). Computational processes represent the steps in GSEs where researchers employ these models to analyze data by computer, encompassing a suite of actions carried out by researchers. These processes form the crux of GSEs, as GSEs are ultimately implemented through the execution of computational processes. Recent advancements in computer technology have facilitated sharing models online to promote resource accessibility and environmental dependency rebuilding, the lack of which are two fundamental barriers to reproduction. In particular, the trend of encapsulating models as web services online is gaining traction. While such service-oriented strategies aid in the reproduction of computational processes, they often ignore the association and interaction among researchers’ actions regarding the usage of sequential resources (model-service resources and data resources); documenting these actions can help clarify the exact order and details of resource usage. Inspired by these strategies, this study explores the organization of computational processes, which can be extracted with a collection of action nodes and related logical links (node-link ensembles). The action nodes are the abstraction of the interactions between participant entities and resource elements (i.e., model-service resource elements and data resource elements), while logical links represent the logical relationships between action nodes. In addition, the representation of actions, the formation of documentation, and the reimplementation of documentation are interconnected stages in this approach. Specifically, the accurate representation of actions facilitates the correct performance of these actions; therefore, the operation of actions can be documented in a standard way, which is crucial for the successful reproduction of computational processes based on standardized documentation. Aprototype system is designed to demonstrate the feasibility and practicality of the proposed approach. By employing this pragmatic approach, researchers can share their computational processes in a structured and open format, allowing peer scientists to re-execute operations with initial resources and reimplement the initial computational processes of GSEs via the open web.

How to cite: Zhu, Z. and Chen, M.: Reproducing computational processes in service-based geo-simulation experiments, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9791, https://doi.org/10.5194/egusphere-egu25-9791, 2025.

EGU25-10981 | Orals | ESSI3.3

yProv: a Software Ecosystem for Multi-level Provenance Management and Exploration in Climate Workflows 

Fabrizio Antonio, Gabriele Padovani, Ludovica Sacco, Carolina Sopranzetti, Marco Robol, Konstantinos Zefkilis, Nicola Marchioro, and Sandro Fiore

Scientific workflows and provenance are two faces of the same medal. While the former addresses the coordinated execution of multiple tasks over a set of computational resources, the latter relates to the historical record of data from its original sources. As experiments rapidly evolve towards complex end-to-end workflows, handling provenance at different levels of granularity and during the entire analytics workflow lifecycle is key for managing lineage information related to large-scale experiments in a flexible way as well as enabling reproducibility scenarios, thus playing a relevant role in Open Science.

The contribution highlights the importance of tracking multi-level provenance metadata in complex, AI-based scientific workflows as a way to foster documentation of data and experiments in a standardized format, strengthen interpretability, trustworthiness and authenticity of the results, facilitate performance diagnosis and troubleshooting activities, and advance provenance exploration. More specifically, the contribution introduces yProv, a joint research effort between CMCC and University of Trento targeting multi-level provenance management in complex, AI-based scientific workflows. The yProv project provides a rich software ecosystem consisting of a web service (yProv service) to store and manage provenance documents compliant with the W3C PROV family of standards, two libraries to track provenance in scientific workflows at different levels of granularity with a focus on AI models training (yProv4WFs and yProv4ML), and a data science tool for provenance inspection, navigation, visualization, and analysis (yProv Explorer). Activity on trustworthy provenance with yProv is also ongoing to fully address end-to-end provenance management requirements.

The contribution will cover the presentation of the yProv software ecosystem and use cases from the interTwin (https://www.intertwin.eu/) and ClimateEurope2 (https://climateurope2.eu/) European projects as well as from the ICSC National Center on HPC, Big Data and Quantum Computing targeting Digital Twins for extreme weather & climate events and data-driven/data-intensive workflows for climate change. 

How to cite: Antonio, F., Padovani, G., Sacco, L., Sopranzetti, C., Robol, M., Zefkilis, K., Marchioro, N., and Fiore, S.: yProv: a Software Ecosystem for Multi-level Provenance Management and Exploration in Climate Workflows, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10981, https://doi.org/10.5194/egusphere-egu25-10981, 2025.

EGU25-11937 | Posters on site | ESSI3.3

DAM2 — A Scalable and Compliant Solution for Managing enriched Infrared images as FAIR Research Data  

Jean Dumoulin, Thibaud Toullier, Nathanael Gey, and Mathias Malandain

Abstract

Efficient and secure dataset management is a critical component of collaborative research projects, where diverse data types, sharing requirements, and compliance regulations converge. This work presents a dataset management tool entitled DAM2 (Data and Model Monitoring) developed within the Chips Joint Undertaking (Chips JU) funded European BRIGHTER project [1], to address these challenges. It provides a robust and adaptable solution for handling private and public ground based measurements datasets throughout the project lifecycle. These datasets combine infrared images (e.g. multispectral ones), with visible images, local weather measurements, labeled data, etc.

The tool is designed to ensure rights management, enabling selective data sharing among authorized partners based on predefined permissions. It incorporates secure access controls to safeguard sensitive data and meets GDPR (General Data Protection Regulation) requirements to guarantee compliance with European privacy standards. For public datasets, the tool integrates with Zenodo, an open-access repository, to support long-term storage and accessibility, aligning with the principles of open science. Key technical features include the usage of an open source, S3 compatible object storage server (MinIO [2]) providing scalability to manage large volumes of data. Additionally, the use of Zarr [3] data format behind the scene offers significant advantages for this cloud-based data management tool, including efficient storage of large datasets through chunking and compression, fast parallel read and write operations, and compatibility with a wide range of data analysis tools. The tool adheres to FAIR (Findable, Accessible, Interoperable, Reusable) principles, storing metadata alongside datasets to enhance usability and interoperability.

Developed as an open-source platform, the tool promotes transparency and collaboration while providing a complete and well-documented API for seamless integration with other systems. A user-friendly interface ensures accessibility for stakeholders with varying technical expertise, while the tool remains flexible to accommodate additional file formats as required. The development process incorporates insights from relevant COFREND (French Confederation for Non-Destructive Testing) working groups, to ensure alignment with broader initiatives in data management, interoperability and durability.

This paper addresses the design, study and developed platform. First operational functionalities are demonstrated through the manipulation of first BRIGHTER and other research project datasets.

In conclusion, DAM2 is a comprehensive solution for managing diverse datasets in collaborative projects, balancing security, compliance, and accessibility. It provides a foundation for efficient, compliant, and interoperable data handling while supporting the principles of open science and FAIR data management.

Perspectives include expanding interoperability with additional repositories, incorporating advanced analytic and visualization features, and integrating AI-driven automation.

Acknowledgments

Authors would like to acknowledge the BRIGHTER HORIZON project. BRIGHTER has received funding from the Chips Joint Undertaking (JU) under grant agreement No 101096985. The JU receives support from the European Union’s Horizon Europe research and innovation program and France, Belgium, Portugal, Spain, Turkey.

References

[1] Brighter --- Project-Brighter. https://project-brighter.eu/, accessed on January 2025.

[2] MinIO, Inc. MinIO S3 Compatible Storage for AI --- Min.Io. https://min.io/, accessed on January, 2025.

[3] Zarr --- Zarr.dev. https://zarr.dev/, accessed on January, 2025.

How to cite: Dumoulin, J., Toullier, T., Gey, N., and Malandain, M.: DAM2 — A Scalable and Compliant Solution for Managing enriched Infrared images as FAIR Research Data , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11937, https://doi.org/10.5194/egusphere-egu25-11937, 2025.

EGU25-13604 | ECS | Orals | ESSI3.3

Streamlining configurations of process-based models through extensible and free workflows 

Kasra Keshavarz, Alain Pietroniro, Darri Eythorsson, Mohamed Ismaiel Ahmed, Paul Coderre, Wouter Knoben, Martyn Clark, and Shervan Gharari

High-resolution and high-complexity process-based hydrological models play a pivotal role in advancing our understanding and prediction of water cycle dynamics, particularly in ungauged basins and under nonstationary climate conditions. However, the configuration, application, and evaluation of these models are often hindered by the intricate and inconsistent nature of a priori information available in various datasets, necessitating extensive preprocessing steps. These challenges can limit the reproducibility, applicability, and accessibility of such models for the broader scientific user community. To address these challenges, we introduce our generalized Model-Agnostic Framework (MAF), aimed at simplifying the configuration and application of data-intensive process-based hydrological models. Through a systematic investigation of commonly used models and their configuration procedures, we provide workflows designed to streamline the setup process for this category of hydrological models. Building on earlier efforts, this framework adheres to the principle of separating model-agnostic and model-specific tasks in the setup procedure of such models. The model-agnostic workflows focus on both dynamic datasets (e.g., meteorological data) and static datasets (e.g., land-use maps), while the model-specific components feed preprocessed, relevant data to the hydrological models of interest. Our initial prototypes of MAF includes recipes for various static and dynamic datasets and also tailored model-specific workflows for MESH, SUMMA, and HYPE process-based modelling frameworks. We demonstrate the effectiveness of these novel workflows in reducing configuration complexity and enhancing the reproducibility of process-based hydrological models through test applications in high-performance computing environments. The framework automates numerous manual tasks, significantly saving time, and enabling continuity in research efforts. Moreover, by minimizing human error and enhancing reproducibility, this research has fostered collaboration with several Canadian government entities, leveraging sophisticated process-based models to address complex environmental challenges.

How to cite: Keshavarz, K., Pietroniro, A., Eythorsson, D., Ahmed, M. I., Coderre, P., Knoben, W., Clark, M., and Gharari, S.: Streamlining configurations of process-based models through extensible and free workflows, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13604, https://doi.org/10.5194/egusphere-egu25-13604, 2025.

EGU25-18040 | ECS | Posters on site | ESSI3.3

Workflows for numerical reproducibility in the OceanVar data assimilation model 

Francesco Carere, Francesca Mele, Italo Epicoco, Mario Adani, Paolo Oddo, Eric Jansen, Andrea Cipollone, and Ali Aydogdu

Numerical reproducibility is a crucial yet often overlooked challenge in ensuring the credibility of computational results and the validity of Earth system models. In large-scale, massively parallel simulations, achieving numerical reproducibility is complicated by factors such as heterogeneous HPC architectures, floating point intricacies, complex hardware/software dependencies, and the non-deterministic nature of parallel execution.

This work addresses the challenges of debugging and ensuring bitwise reproducibility (BR) in parallel simulations, specifically for the MPI-parallelised OceanVar data assimilation model. We explore methods for detecting and resolving BR-related bugs, focusing on an automated debugging process. Currently mature tools to automate this process are lacking for bugs due to MPI-parallelisation, making automatic BR verification in scientific workflows involving such codebases a time-consuming challenge.

However, BR is sometimes considered unrealistic in workflows involving heterogeneous computing architectures. As an alternative, statistical reproducibility (SR) is proposed and explored by various research groups in the Earth system modelling community, for which automated tools have been developed. For example, the scientific workflow of CESM supports automatic verification of SR using the CESM-ECT framework/PyCECT software. In case of failure of SR a root-cause analysis tool exists, CESM-RUANDA, albeit currently not fully functional. We explore SR as an alternative and complementary approach to of BR focusing on its potential to support numerical reproducibility in workflows involving heterogeneous computing architectures.

How to cite: Carere, F., Mele, F., Epicoco, I., Adani, M., Oddo, P., Jansen, E., Cipollone, A., and Aydogdu, A.: Workflows for numerical reproducibility in the OceanVar data assimilation model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18040, https://doi.org/10.5194/egusphere-egu25-18040, 2025.

EGU25-18890 | Posters on site | ESSI3.3

Research data management for numerical simulations in Earth-System Science 

Klaus Getzlaff and Markus Scheinert

One of today's challenges is the effective access to scientific data either within research groups or across different institutions to increase the reusability of the data and therefore their value. While large operational modeling and service centers have enabled query and access to data via common web services, this is often not the case for smaller institutions or individual research groups. Especially the maintenance of the infrastructure and the simplicity of the workflows, in order to make the data and their provenance available and accessible, are common challenges for scientists and data management.

At GEOMAR there are several data steward positions to support RDM for special disciplines and formats. They are also connected across centres to work on common standards, e.g. the netcdf standard working group in the Helmholtz Earth and Environment DataHUB.

Here we will present the institutional approach on research data management for numerical simulations in earth system science. The data handling, especially the possibilities for data sharing, publication and access, which is in today’s focus, is realized by using persistent identifier handles in combinations with a modern http web server index solution and a THREDDS server allowing remote access using standardized protocols such as OPeNDAP, WMS. By cross-linking this into the central institutional metadata and publication repositories it allows the re-usability of the data by scientists from different research groups and backgrounds. In addition to the pure data handling the documentation of the numerical simulation experiments is of similar importance to allow re-usability or reproducibility and to provide the data which will be addressed too.

How to cite: Getzlaff, K. and Scheinert, M.: Research data management for numerical simulations in Earth-System Science, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18890, https://doi.org/10.5194/egusphere-egu25-18890, 2025.

EGU25-19655 | Posters on site | ESSI3.3

Multi-faceted habitat connectivity: how to orchestrate remote sensing with citizen science data? 

Ivette Serral, Vitalii Kriukov, Lucy Bastin, Riyad Rahman, and Joan Masó

In the era of declining biodiversity, global climate change and transformations in land use, terrestrial habitat connectivity is one of the key parameters of ecosystem management. In this regard, the land-use/land-cover (LULC) dynamics is crucial to detect the spatiotemporal trends in connectivity of focal endangered species and to predict the effects for biodiversity for planned or proposed LULC changes.

Apart from the LULC derivatives of remote sensing, connectivity analysis and scenarios modelling can also benefit from citizen science datasets, such as Open Street Map and GBIF species occurrence data cubes in which aggregated data can be perceived as a cube with three dimensions - taxonomic, temporal and geographic. The synthetic LULC datasets which cover Catalonia every 5 years (1987-2022) were enriched via developed Data4Land harmonisation tool harnessing Open Street Map (through Overpass Turbo API) and World Database on Protected Areas. Two outstanding well-known tools, Graphab and MiraMon GIS&RS (using the Terrestrial Connectivity Index Module - ICT), were used to create the overarching dataset on terrestrial habitat connectivity in Catalonia (2012-2022) for target species and broad land cover categories, forests. Significant decline trends in forest habitat connectivity are observed for Barcelona metropolitan area, and vice versa in the Pyrenees mountain corridor and protected areas. According to the local case study on the connectivity of Mediterranean turtle in the Albera Natural Park, general positive trend was affected by massive fires in 2012.

To ensure the replicable results, the pipeline to create reliable metadata in accordance with FAIR principles, especially data lineage, is being developed, as well as the high performance computing pipeline for Graphab.

How to cite: Serral, I., Kriukov, V., Bastin, L., Rahman, R., and Masó, J.: Multi-faceted habitat connectivity: how to orchestrate remote sensing with citizen science data?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19655, https://doi.org/10.5194/egusphere-egu25-19655, 2025.

EGU25-21553 | Posters on site | ESSI3.3

European Digital Twin of the Ocean: the integration with EuroHPC platforms 

Stella Valentina Paronuzzi Ticco, Simon Lyobard, Mathis Bertin, Quentin Gaudel, Jérôme Gasperi, and Alain Arnaud

The EDITO platform serves as the foundational framework for building the European Digital Twin of the Ocean, seamlessly integrating oceanographic data, processes and services on a single and comprehensive platform. The platform provides scalable computing resources interconnected with EuroHPC supercomputing centers. We have developed a mechanism that allows users to remotely execute functions (processes) on HPCs and store the resulting output at the location of their choice (e.g. EDITO personal storage, third parties S3 buckets, etc.). This output can then be leveraged as input for subsequent processes, fostering a streamlined and interconnected workflow. Our presentation will delve into the technical details to achieve such an integration between cloud and HPC systems. 

How to cite: Paronuzzi Ticco, S. V., Lyobard, S., Bertin, M., Gaudel, Q., Gasperi, J., and Arnaud, A.: European Digital Twin of the Ocean: the integration with EuroHPC platforms, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21553, https://doi.org/10.5194/egusphere-egu25-21553, 2025.

EGU25-1294 | Posters on site | ESSI2.13

A new sub-chunking strategy for fast netCDF-4 access in local, remote and cloud infrastructures.  

Flavien Gouillon, Cédric Penard, Xavier Delaunay, and Sylvain Herlédan

NetCDF (Network Common Data Form) is a self-describing, portable and platform-independent format for array-oriented scientific data which has become a community standard for sharing measurements and analysis results in the fields of oceanography, meteorology but also in the space domain.

The volume of scientific data is continuously increasing at a very fast rate. Object storage, a new paradigm that appeared with cloud infrastructures, can help with data storage and parallel access issues, but NetCDF may not be able to get the most out of this technology without some tweaks and fine tuning.

The availability of ample network bandwidth within cloud infrastructures allows for the utilization of large amounts of data. Processing data       where the data is located is preferable as it can result in substantial resource savings. But for some use cases downloading data from the cloud is required (e.g. processing also involving confidential data) and results still have to be fetched once processing tasks have been executed on the cloud.

Networks      exhibit significant variations in capacity and quality (ranging from fiber-optic and copper connections to satellite connections with poor reception in degraded conditions on boats, among other scenarios). Therefore, it is crucial for formats and software libraries to be specifically designed to optimize access to      data by minimizing the transfer to only what is strictly necessary.

In this context, a new approach has emerged in the form of a library that indexes the content of netCDF-4 datasets. This indexing enables the retrieval of sub-chunks, which are pieces of data smaller than a chunk, without the need to reformat the existing files. This approach targets access patterns such as time series in netCDF-4 datasets formatted with large chunks.

This report provides a performance assessment of netCDF-4 datasets for varied use cases. This assessment executes these use cases under various conditions, including POSIX and S3 local filesystems, as well as a simulated degraded network connection. The results of this assessment may provide guidance on the most suitable and most efficient library for reading netCDF data in different situations.

How to cite: Gouillon, F., Penard, C., Delaunay, X., and Herlédan, S.: A new sub-chunking strategy for fast netCDF-4 access in local, remote and cloud infrastructures. , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1294, https://doi.org/10.5194/egusphere-egu25-1294, 2025.

EGU25-4155 | Orals | ESSI2.13

How open software, data and platforms are transforming Earth observation data science 

Wolfgang Wagner, Matthias Schramm, Martin Schobben, Christoph Reimer, and Christian Briese

One of the most time-consuming and cumbersome tasks in Earth observation data science is finding, accessing and pre-processing geoscientific data generated by satellites, ground-based networks, and Earth system models. While the much increased availability of free and open Earth observation datasets has made this task easier in principle, scientific standards have evolved according to data availability, now emphasizing research that integrates multiple data sources, analyses longer time series, and covers larger study areas. As a result of this “rebound effect”, scientists and students may find themselves spending even more of their time on data handling and management than in the past. Fortunately, cloud platform services such as Google Earth Engine can save significant time and effort. However, until recently, there were no standardized methods for users to interact with these platforms, meaning that code written for one service could not easily be transferred to another (Schramm et al., 2021). This created a dilemma for many geoscientists: should they use proprietary cloud platforms to save time and resources at the risk of lock-in effects, or rely on publicly-funded collaborative scientific infrastructures, which require more effort for data handling? In this contribution, we argue that this dilemma is about to become obsolete thanks to rapid advancements in open source tools that allow building open, reproducible, and scalable workflows. These tools facilitate access to and integration of data from various platforms and data spaces, paving the way for the “Web of FAIR data and services” as envisioned by the European Open Science Cloud (Burgelman, 2021). We will illustrate this through distributed workflows that connect Austrian infrastructures with European platforms like the Copernicus Data Space Ecosystem and the DestinE Data Lake (Wagner et al., 2023). These workflows can be built using Pangeo-supported software libraries such as Dask, Jupyter, Xarray, or Zarr (Reimer et al., 2023). Beyond advancing scientific research, these workflows are also valuable assets for university education and training. For instance, at TU Wien, Jupyter notebooks are increasingly used in exercises involving Earth observation and climate data, and as templates for student projects and theses. Building on these educational resources, we are working on an Earth Observation Data Science Cookbook to be published on the Project Pythia website, a hub for education and training in the geoscientific Python community.

References

Burgelman (2021) Politics and Open Science: How the European Open Science Cloud Became Reality (the Untold Story). Data Intelligence 3, 5–19. https://doi.org/10.1162/dint_a_00069

Reimer et al. (2023) Multi-cloud processing with Dask: Demonstrating the capabilities of DestinE Data Lake (DEDL), Conference on Big Data from Space (BiDS’23), Vienna, Austria. https://doi.org/0.2760/46796

Schramm et al. (2021) The openEO API–Harmonising the Use of Earth Observation Cloud Services Using Virtual Data Cube Functionalities. Remote Sensing 13, 1125. https://doi.org/10.3390/rs13061125

Wagner et al. (2023) Federating scientific infrastructure and services for cross-domain applications of Earth observation and climate data, Conference on Big Data from Space (BiDS’23), Vienna, Austria. https://doi.org/10.34726/5309

How to cite: Wagner, W., Schramm, M., Schobben, M., Reimer, C., and Briese, C.: How open software, data and platforms are transforming Earth observation data science, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4155, https://doi.org/10.5194/egusphere-egu25-4155, 2025.

EGU25-4277 | Posters on site | ESSI2.13

BEACON Binary Format (BBF) - Optimizing data storage and access to large data collections 

Tjerk Krijger, Peter Thijsse, Robin Kooyman, and Dick Schaap

As part of European projects, such as EOSC related Blue-Cloud2026, EOSC-FUTURE and FAIR-EASE, MARIS has developed and demonstrated a software system called BEACON with a unique indexing system that can, on the fly with high performance, extract data subsets based on the user’s request from millions of heterogeneous observational data files. The system returns one single harmonised file as output, regardless of whether the input contains many different data types or dimensions. 

Since in many cases the original data collections that are imported in a BEACON installment contain millions of files (e.g. Euro-Argo, SeaDataNet, ERA5, World Ocean Database), it is hard to achieve fast responses. Next to this, these large collections also require a large storage capacity. To mitigate these issues, we wanted to optimize the internal file format that is used within BEACON. With the aim of reducing the data storage size and speeding up the data transfer, while guaranteeing that the information of the original data files is maintained. As a result, the BEACON software has included a unique file format called the “BEACON Binary Format (BBF)” that meets these requirements. 

The BBF is a binary data format that allows for storing multi-dimensional data as apache arrow arrays with zero deserialization costs. This means that computers can read the data stored on disk, as if it were computer memory, significantly reducing computational access time by eliminating the cost for a computer to translate what’s on disk, to computer memory.

Together with making the entire data format “non-blocking”, which means that all computer cores can access the file at the same time and simultaneously use the jump table to read millions of datasets in parallel. This enables a level of performance which reaches speeds of multiple GB/s, making the hardware the bottleneck instead of the software.

Furthermore, the format takes a unique approach to compressing data by adjusting the way it compresses and decompresses on a per dataset level. This means that every dataset is compressed in a slightly different manner, making it much more effective in terms of size reduction and time to decompress the data which can get close to the effective memory speed of a computer.

It does this while retaining full data integrity. No data is ever lost within this format, nor is any data adjusted. If one were to import a NetCDF file into BBF, one could fully rebuild the original NetCDF file from the BBF file itself. In the presentation the added benefits of using the BBF will be highlighted by comparing and benchmarking it to traditional formats such as NetCDF, CSV, ASCII, etc.

In January 2025, BEACON 1.0.0 was made publicly available as an open-source software, allowing everyone to set-up their own BEACON node to enhance the access to their data, while at the same time being able to reduce the storage size of their entire data collection without losing any information. More technical details, example applications and general information on BEACON can be found on the website https://beacon.maris.nl/.

How to cite: Krijger, T., Thijsse, P., Kooyman, R., and Schaap, D.: BEACON Binary Format (BBF) - Optimizing data storage and access to large data collections, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4277, https://doi.org/10.5194/egusphere-egu25-4277, 2025.

EGU25-5977 | Orals | ESSI2.13

A comparative study of algorithms for lossy compression of 2-d meteorological gridded fields 

Uwe Ehret, Jieyu Chen, and Sebastian Lerch

Meteorological observations (e.g. from weather radar) and the output of meteorological models (e.g. from reanalyses or forecasts) are often stored and used in the form of time series of 2-d spatial gridded fields. With increasing spatial and temporal resolution of these products, and with the transition from providing single deterministic fields to providing ensembles, their size has dramatically increased, which makes use, transfer and archiving a challenge. Efficient compression of such fields - lossy or lossless - is required to solve this problem.

The goal of this work was therefore to apply several lossy compression algorithms for 2d spatial gridded meteorological fields, and to compare them in terms of compression rate and information loss compared to the original fields. We used five years of hourly observations of rainfall and 2m air temperature on a 250 x 400 km region over central Germany on a 1x1 km grid for our analysis.

In particular, we applied block averaging as a simple benchmark method, Principal Component Analysis, Autoencoder Neural Network (Hinton and Salakhutdinov, 2006) and the Ramer-Douglas-Peucker algorithm (Ramer, 1972; Douglas and Peucker, 1973) known from image compression. Each method was applied for various compression levels, expressed as the number of objects of the compressed representation, and then the (dis-)similarity of the original field and the fields reconstructed from the compressed fields was measured by Mean Absolute Error, Mean Square Error, and the Image Quality Index (Wang and Bovik, 2002). First results indicate that even for spatially heterogeneous fields like rainfall, very high compression can be achieved with small error.

 

References

Douglas, D., Peucker, T.: Algorithms for the reduction of the number of points required to represent a digitized line or its caricature. In: The Canadian Cartographer. Bd. 10, Nr. 2, 1973, ISSN 0008-3127, S. 112–122, 1973.

Hinton, G. E., & Salakhutdinov, R. R.: Reducing the dimensionality of data with neural networks. science, 313(5786), 504-507, 2006.

Ramer, U.: An iterative procedure for the polygonal approximation of plane curves, Computer Graphics and Image Processing, 1, 244-256, http://dx.doi.org/10.1016/S0146-664X(72)80017-0, 1972.

Zhou Wang, and A. C. Bovik: A universal image quality index, IEEE Signal Processing Letters, 9, 81-84, 10.1109/97.995823, 2002.

How to cite: Ehret, U., Chen, J., and Lerch, S.: A comparative study of algorithms for lossy compression of 2-d meteorological gridded fields, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5977, https://doi.org/10.5194/egusphere-egu25-5977, 2025.

EGU25-7371 | ECS | Orals | ESSI2.13

Evaluating Advanced Scientific Compressors on Climate Datasets 

Robert Underwood, Jinyang Liu, Kai Zhao, Sheng Di, and Franck Cappello

    As climate and weather scientists strive to increase accuracy and understanding of our world, models of weather and climate have increased in their resolution to square kilometers scale and become more complex increasing their demands for data storage. A recent study SCREAM run at 3.5km resolution produced nearly 4.5TB of data per simulated day, and the recent CMIP6 simulations produced nearly 28PB of data. At the same time, storage and power capacity at facilities conducting climate experiments are not increasing at the same rate as the volume of climate and weather datasets leading to a pressing challenge to reduce data volumes. While some in the weather and climate community have adopted lossless compression, these techniques frequently produce compression ratios on the order of 1.3$\times$, which are insufficient to alleviate storage constraints on facilities. Therefore, additional techniques, such as science-preserving lossy compression that can achieve higher compression ratios, are necessary to overcome these challenges.

    While data compression is an important topic for climate and weather applications, many of the current assessments of the effectiveness of climate and weather datasets do not consider the state of the art in compressor design and instead, asses scientific compressors that are 3-11 years old, substantially behind the state of the art. In this report: 

 

  •  We assess the current state of the art in advanced scientific lossy compressors against the state of the art in quality assessment criteria proposed for the ERA5 dataset to assess the current gaps between needed performance requirements and the capabilities of the current compressors.
  • We present new capabilities that allow us to build an automated, user-friendly, and extensible pipeline for quickly finding compressor configurations that maximize compression ratios while preserving scientific integrity of the data using codes developed as part of the NSF FZ project.
  • We demonstrate a number of capabilities that facilitate use within in the weather and climate community including NetCDF, HDF5, and GRIB file format support; support for innovation via Python, R, and Julia as well as low level languages such as C/C++; and the implementations of commonly used climate quality metrics including dSSIM, and the ability to extend to add new metrics in high-level languages
  • Utilizing this pipeline, We find that with advanced scientific compressors, it is possible to achieve a 6.4x improvement or more in compression ratio over previously evaluated compressors

How to cite: Underwood, R., Liu, J., Zhao, K., Di, S., and Cappello, F.: Evaluating Advanced Scientific Compressors on Climate Datasets, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7371, https://doi.org/10.5194/egusphere-egu25-7371, 2025.

EGU25-11118 | Orals | ESSI2.13

Too Big to Handle? Hexagonizing LIDAR and Satellite Data in Geoscience Applications 

Bo Møller Stensgaard, Casper Bramm, Marie Katrine Traun, and Søren Lund Jensen

The exponential growth of LIDAR and satellite data in geoscience presents both opportunities and challenges for users. Traditional data handling methods often struggle with the sheer volume and complexity of these datasets, hindering easy accessibility, efficient analysis and decision-making processes. This presentation introduces the Scandinavian Highlands HEX-Responder platform and database structure, a cutting-edge solution that leverages the power of hexagonal discrete global grid system, Uber H3, and developed processes to revolutionize geospatial data management, fast responsive visualization and analysis.

We will showcase real-world applications, highlighting the platform's potential to accelerate scientific discovery and improve decision-making processes using satellite and remote sensing data.

The platform’s approach offers several advantages over conventional methods:

  • Efficient data organization and retrieval
  • Improved advanced spatial data analyses opportunities
  • Seamless integration of multi-scale and multi-dimensional data without losing information
  • Enhanced, responsive and fast visualisation capabilities

Our ELT (extract, load, transform) and subsequent visualisation procedure can be applied to any big raster data formats. First, the raw raster data is transformed into optimised parquet files through chunked reading and compression based on a low-resolution H3 hexagon cell index (hexagonization), enabling rapid data import to a column-oriented database management system for big data storage, processing and analytics. The H3 cell organisation is preserved in the database through partitioned fetching for visualisation on the platform. This method allows for horizontal scaling and accurate multi-resolution aggregation, preserving data integrity across scales and significantly overcomes typical computational memory limitations.

The platform's capabilities are exemplified by its approach to LIDAR and satellite emissivity data processing using the H3 grid. High-resolution LIDAR data is efficiently gridded and visualized to H3 resolution level 15 hexagons (0.9m2 hexagon cells). The gridding preserves all original pixel raster points while providing aggregated views for seamless zooming.

Another prime example of the capabilities is the handling of NASA’s ASTER Global Emissivity Data (100m resolution). Here, our pipeline transformed 2.1 terabytes of extracted raw CSV-data derived from NASA’s emissivity data into a compressed format based on the H3 index occupying only 593 gigabytes in the database.

This approach not only saves data storage space but also dramatically improves data accessibility and processing speed for the users, allowing users to work in a responsive environment with this massive dataset in ways previously not possible. Each hexagon represents an opportunity to store unlimited amount, types and categories of pre-processed data for more integrative analyses and data insight.

By hexagonizing LIDAR and satellite data, the HEX-Responder platform enables users to explore massive datasets with ease and efficiency in a responsive environment. The integrated procedures allow for detailed information maintenance and retrieval, paving the way for advanced predictive modelling in geoscience applications using earth observation data in a new way.  

How to cite: Stensgaard, B. M., Bramm, C., Traun, M. K., and Jensen, S. L.: Too Big to Handle? Hexagonizing LIDAR and Satellite Data in Geoscience Applications, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11118, https://doi.org/10.5194/egusphere-egu25-11118, 2025.

EGU25-12760 | ECS | Posters on site | ESSI2.13

Tree-Based Adaptive Data Reduction Techniques for Scientific Simulation Data 

Niklas Böing, Johannes Holke, Achim Basermann, Gregor Gassner, and Hendrik Fuchs

Large-scale Earth system model simulations produce huge amounts of data. Due to limited I/O bandwidth and available storage space this data often needs to be reduced before written to disk or stored permanently. Error-bounded lossy compression is an effective approach to tackle the trade-off between accuracy and storage space.

We are exploring and discussing lossless as well as error-bounded lossy compression based on tree-based adaptive mesh refinement/coarsening (AMR) techniques. Our lossy compression schemes allow for absolute and relative error bounds. The data reduction methods are closely linked to an underlying (adaptive) mesh which easily permits error regions of different error tolerances and criteria – in particular, we allow nested domains of varying error tolerances specified by the user. Moreover, some of the compressed data structures allow for an incremental decompression in the resolution of the data which may be favorable for transmission and visualization.

We implement these techniques as the open source tool cmc, which is based on the parallel AMR library t8code. The compression tool can be linked to and used by arbitrary simulation applications or executed as a post-processing step. We show different application results of the compression in comparison to current state-of-the-art compression techniques on several benchmark data sets.

How to cite: Böing, N., Holke, J., Basermann, A., Gassner, G., and Fuchs, H.: Tree-Based Adaptive Data Reduction Techniques for Scientific Simulation Data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12760, https://doi.org/10.5194/egusphere-egu25-12760, 2025.

EGU25-13394 | ECS | Orals | ESSI2.13

Challenges and perspectives of climate data compression in times of kilometre-scale models and generative machine learning 

Milan Klöwer, Tim Reichelt, Juniper Tyree, Ayoub Fatihi, and Hauke Schulz

Climate data compression urgently needs new standards. The continuously growing exascale mountain of data requires compressors that are widely used and supported, essentially hiding the compression details from many users. With the advent of AI revolutionising scientific computing, we have to set the rules of this game. Minimizing information loss, maximising compression factors, at any resolution, grid and dataset size, for all variables, with chunks and random access, while preserving all statistics and derivatives, at a reasonable speed — are squaring the compression circle. Many promising compressors are hardly used as trust among domain scientists is hard to gain: The large spectrum of research questions and applications using climate data is very difficult to satisfy simultaneously.

Here, we illustrate the motivation behind the newly defined climate data compression benchmark ClimateBenchPress, designed as a quality check in all those dimensions of the problem. Any benchmark will inevitably undersample this space, but we define datasets from atmosphere, ocean, and land as well as evaluation metrics to pass. Results are presented as score cards, highlighting strengths and weaknesses for every compressor.

The bitwise real information content shows a systematic way in case no error bounds are known. In the case of the ERA5 reanalysis, errors are estimated and allow us to categorize many variables into linear, log and beta distributions with values bounded from zero, one or both sides, respectively. This allows us to define error thresholds arising from observation and model errors directly, providing another alternative to the still predominant subjective choices. Most error-bounded compressors come with parameters that can be automatically chosen following this analysis.

Also new data formats are on the horizon: Chunking and hierarchical data structures allow and force us to adapt compressors to spatially or length-scale dependent information densities. Extreme events, maybe counterintuitively, often increase the compressibility through higher uncertainties, but lie on the edge or outside of the training data for machine learned-compressors. This again increases the need for well-tested compressors. Benchmarks like ClimateBenchPress are required to encourage new standards for safe lossy climate data compression.

How to cite: Klöwer, M., Reichelt, T., Tyree, J., Fatihi, A., and Schulz, H.: Challenges and perspectives of climate data compression in times of kilometre-scale models and generative machine learning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13394, https://doi.org/10.5194/egusphere-egu25-13394, 2025.

EGU25-13567 | Posters on site | ESSI2.13

Tables as a way to deal with a variety of data formats and APIs in data spaces 

Joan Masó, Marta Olivé, Alba Brobia, Nuria Julia, Nuria Cartell, and Uta Wehn

The Green Deal Data Space is born in the big data paradigm where there is a variety of data formats and data models that are exposed as files or web APIs. As a result, we need to default in simple data structure that is transversal enough to be able to represent most of the more specific data models, formats and API payloads. Many data models present a structure that can be represented as tables.

TAPIS stands for "Tables from APIS". It is a JavaScript code that uses a common data model that is an array of objects with a list of properties that can contain a simple or a complex value. In TAPIS offers a series of operations that use one or more arrays of objects as inputs and produce a new array of objects as an output. There are operations that create the arrays of objects from files or API queries (a.k.a. data import), others that manipulate the objects (e.g. merge two arrays in a single one) and some operations that generate visual representations of the common data structure including tabular, a map, a graph, etc.

TAPIS is limited by its own data model. While many of the data models can be mapped to the common data model, a multidimensional data cube or a data tree cannot be represented in a single table in an efficient way. In the context of the Green Deal Data Space, most of the sensor data, statistical data, geospatial feature based data and administrative data can be considered object based data and can be used in TAPIS. TAPIS is able to connect to Sensor Things API (the sensor protocol selected in AD4GD and CitiObs), S3 buckets (the internal cloud repository used in AD4GD), GeoNetwork (the geospatial metadata catalogue selected in AD4GD and more4nature), and the OGC API features and derivates (the modern web API interfaces standardized by the OGC) but other data inputs will be incorporated, such as Citizen Science data sources and other popular APIs used in the more4nature project. More analytical functionalities are going to be incorporated in the CitiObs project. As part of the AD4GD Green Deal Information Model, there is an operation to associate semantics to each column of a table by linking it to a URI that defines the concept in an external vocabulary (as well as units of measure if appropriate). In order to be compatible with the data space architecture recommended by the International Data Space Association, we are working on supporting the catalogue of the Eclipse Data Connector, and to be able to negotiate a digital contract as a previous step to request access to the relevant data offered in the data space. To do so, we are working on incorporating the data space protocol as part of the TAPIS operations for data import. TAPIS is available as open source at https://github.com/joanma747/TAPIS.

AD4GD, CitiObs and more4nature are Horizon Europe projects co-funded by the European Union, Switzerland and the United Kingdom.

How to cite: Masó, J., Olivé, M., Brobia, A., Julia, N., Cartell, N., and Wehn, U.: Tables as a way to deal with a variety of data formats and APIs in data spaces, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13567, https://doi.org/10.5194/egusphere-egu25-13567, 2025.

Early career scientists rarely have the resources to work with earth observation data at continental to global scale. This is caused by a combination of factors: large scale data analysis often involves teamwork, connecting data scientists, code developers, IT specialists, statisticians and geoscientists. Young researchers are rarely able to coordinate such a team. Meanwhile, all scientists can have relevant ideas or pose powerful research questions that merit investigation. Copernicus Data Space Ecosystem provides a public, free platform for large-scale processing of earth observation data. It combines instant access to all Sentinel satellite imagery with cloud-based processing in the form of API requests and a powerful browser-based viewing interface. This new approach is enabled by storing the data in a different way: uncompressed formats such as JPEG2000, COG or ZARR support subsetting and querying the image rasters without first unzipping the file, thereby allowing direct streaming of only the area and bands that the user requests. Additionally, this means that most calculations and visualization tasks can be carried out on the server side, directly within the request process. The backend tasks of data storage and management are taken care of by the system, while the user can concentrate on the research itself.

Copernicus Data Space Ecosytem supports several API families. OGC API-s directly enable the creation of Open Geospatial Consortium compatible map products such as WMS, WMTS, WFS or WCS services. These can be accessed with GIS software or displayed in web map tools. OData, STAC, and OpenSearch are Catalog API-s, supporting the querying and of datasets in preparation for analysis. Sentinel Hub is an API family that can handle queries, raster operations, and raster-vector integration for deriving statistics. The main advantages of Sentinel Hub API-s are their efficient use and integration with advanced visualization in the Copernicus Browser.

OpenEO is a fully open-source data analysis framework designed specifically to support FAIR principles. It is independent from data formats with its own data cube format, and can be edited using several coding languages. openEO connects to all STAC-compliant repositories, enabling integration between Sentinel data and other sources. Processing tools include many mathematical operations, but also standard machine learning processes. The system is designed with upscaling in mind: the command structure is the same for small and large areas, with storage and asynchronous processing managed by the backend.

Both API families come with a comprehensive scheme of tutorials and documentation to allow step-by-step learning, and an online Jupyter Lab virtual machine facility. Therefore, early-career scientists with a basic understanding of programming can quickly learn to apply their domain knowledge, while creating solutions that are easy to share and replicate.

All in all, Copernicus Data Space Ecosystem is a transformative tool for earth observation, significantly lowering the bar for applying earth observation at large scale in the geosciences.

How to cite: Zlinszky, A. and Milcinski, G.: Copernicus Data Space Ecosystem empowers early-career scientists to do global scale earth observation data analysis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15282, https://doi.org/10.5194/egusphere-egu25-15282, 2025.

EGU25-15672 | ECS | Posters on site | ESSI2.13

Scaling Down ESS Datasets: Lessons from the EERIE Project on Compression 

Oriol Tinto, Xavier Yepes, and Pierre Antoine Bretonniere

The rapid growth of Earth System Sciences (ESS) datasets, driven by high-resolution numerical modeling, has outpaced storage and data-sharing capabilities. To address these challenges, we investigated lossy compression techniques as part of the EERIE project, aiming to significantly reduce storage demands while maintaining the scientific validity of critical diagnostics.

Our study examined two key diagnostics: Sea Surface Height (SSH) variability and ocean density, essential for understanding climate dynamics. Leveraging tools such as SZ3 and enstools-compression, we achieved data volume reductions by orders of magnitude without compromising the diagnostics' accuracy. Compression-induced differences were found to be negligible compared to the inherent variability between model outputs and observational datasets, underscoring the robustness of these methods.

Additionally, our work highlighted inefficiencies in current workflows, including the prevalent use of double precision in post-processing. We proposed improvements to align data precision with the original model outputs, further optimizing storage and computation. Integrating lossy compression into existing workflows via widely used formats like NetCDF and HDF5 demonstrates a practical path forward for sustainable ESS data management.

This study showcases the transformative potential of lossy compression to make high-resolution datasets more manageable, ensuring they remain accessible and scientifically reliable for stakeholders while significantly reducing resource demands.

How to cite: Tinto, O., Yepes, X., and Bretonniere, P. A.: Scaling Down ESS Datasets: Lessons from the EERIE Project on Compression, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15672, https://doi.org/10.5194/egusphere-egu25-15672, 2025.

EGU25-15864 | Posters on site | ESSI2.13

The Sentinels EOPF Toolkit: Driving Community Adoption of the Zarr data format for Copernicus Sentinel Data 

Sabrina H. Szeto, Julia Wagemann, Emmanuel Mathot, and James Banting

The Standard Archive Format for Europe (SAFE) specification has been the established approach to publishing Copernicus Sentinel data products for over a decade. While SAFE has pushed the ecosystem forward through new ways to search and access the data, it is not ideal for processing large volumes of data using cloud computing. Over the last few years, data standards like STAC and cloud-native data formats like Zarr and COGs have revolutionised how scientific communities work with large-scale geospatial data and are becoming a key component of new data spaces, especially for cloud-based systems.

The ESA Copernicus Earth Observation Processor Framework (EOPF) will be providing access to “live” sample data from the Copernicus Sentinel missions -1, -2 and -3 in the new Zarr data format. This set of reprocessed data allows users to try out accessing and processing data in the new format and experiencing the benefits thereof with their own workflows.

This presentation introduces a community-driven toolkit that facilitates the adoption of the Zarr data format for Copernicus Sentinel data. The creation of this toolkit was driven by several motivating questions: 

  • What common challenges do users face and how can we help them overcome them? 
  • What resources would make it easier for Sentinel data users to use the new Zarr data format? 
  • How can we foster a community of users who will actively contribute to the creation of this toolkit and support each other?

The Sentinels EOPF Toolkit team, comprising Development Seed, SparkGeo and thriveGEO, together with a group of champion users (early-adopters), are creating a set of Jupyter Notebooks and plug-ins that showcase the use of Zarr format Sentinel data for applications across multiple domains. In addition, community engagement activities such as a notebook competition and social media outreach will bring Sentinel users together and spark interaction with the new data format in a creative yet supportive environment. Such community and user adoption efforts are necessary in order to overcome adoption and uptake barriers and to build up trust and excitement to try out new technologies and new developments around data spaces.

In addition to introducing the Sentinels EOPF Toolkit, this presentation will also highlight lessons learned from working closely with users on barriers they face in adopting the new Zarr format and how to address them. 

How to cite: Szeto, S. H., Wagemann, J., Mathot, E., and Banting, J.: The Sentinels EOPF Toolkit: Driving Community Adoption of the Zarr data format for Copernicus Sentinel Data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15864, https://doi.org/10.5194/egusphere-egu25-15864, 2025.

EGU25-16791 | ECS | Posters on site | ESSI2.13

Development and performance evaluation of dissolved oxygen climatology in the Northwestern Pacific 

Jae-Ho Lee, Yong Sun Kim, and Sung-Dae Kim

This study developed a monthly regional atlas for dissolved oxygen (DO) with a quarter-degree horizontal resolution and 73 vertical levels over the northwestern Pacific. We used observed profiles of 586,851 and gridded World Ocean Atlas 2023 (WOA23) with 1° resolution by adopting simple kriging horizontal interpolation and vertical stabilizing techniques to produce the new atlas. This approach efficiently mitigates artificial water masses and statistical noise. The new DO climatology provides detailed information along coasts and renders realistic oxygen distribution associated with the current system in the western North Pacific compared to WOA23. A meridional section demonstrates that the newly developed atlas does not yield artificial noise-like spikes frequently observed in WOA23 in the East Sea. This study expects that this new atlas can allow bio-geochemical numerical models to enhance diagnostic and forecasting performance.

How to cite: Lee, J.-H., Kim, Y. S., and Kim, S.-D.: Development and performance evaluation of dissolved oxygen climatology in the Northwestern Pacific, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16791, https://doi.org/10.5194/egusphere-egu25-16791, 2025.

EGU25-17102 | Posters on site | ESSI2.13

Calculation of Gridded Surface Current from Observed Lagrangian Trajectories in the East Sea 

Mi-Jin Jang, Jae-Ho Lee, and Yong Sun Kim

Surface ocean current is crucial for enhancing the safety and efficiency of maritime logistics and transportation, boosting fisheries production and management, and supporting military operations. This study analyzed 25,342 trajectories from NOAA’s Global Drifter Program (1991–2020), 12 from KIOST, and 63 from KHOA (2015–2024). The surface drifters entering the East Sea were extracted, and a five-step quality control process was implemented. Unobserved values were removed, quality control was applied based on drogue lost, abnormally speed or stuck, unrealistic acceleration. To estimated the gridded oceanic current with high-resolution, we removed the Ekman current and tides from the observed velocity and took advantage of a simple kriging approach. The validation against existing datasets confirmed that major ocean currents exhibited similar patterns compared to absolute geostrophic current from the satellite-based altimetry. The constructed dataset is expected to contribute to the accurate identification of surface current movements and the development of realistic models that incorporate regional characteristics based on data assimilation.

How to cite: Jang, M.-J., Lee, J.-H., and Kim, Y. S.: Calculation of Gridded Surface Current from Observed Lagrangian Trajectories in the East Sea, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17102, https://doi.org/10.5194/egusphere-egu25-17102, 2025.

The Copernicus Program is the largest and most successful public space program globally. It provides continuous data across various spectral ranges, with an archive exceeding 84 petabytes and a daily growth of approximately 20 TB, both of which are expected to increase further. The openness of its data has contributed to the widespread use of Earth observation and the development of commercial products utilizing open data in Europe and worldwide. The entire archive, along with cloud-based data processing capabilities, is available free of charge through the Copernicus Data Space Ecosystem initiative and continues to evolve to meet global user standards. 

This paper presents the process of creating the STAC Copernicus Data Space Ecosystem catalog—the largest and most comprehensive STAC catalog in terms of metadata globally. It details the workflow, starting from the development of a metadata model for Sentinel data, through efficient indexing based on the original metadata files accompanying the products, to result validation and backend system ingestion (via database DSN). A particular highlight is that this entire process is executed using a single tool, eometadatatool, initially developed by DLR, further enhanced, and released as open-source software by the CloudFerro team. The eometadatatool facilitates metadata extraction from the original files accompanying Copernicus program products and others (e.g., Landsat, Copernicus Contributing Missions) using a CSV file containing the metadata name, the file in which it occurs, and the path to the key within the file. Since the CDSE repository operates as an S3 resource offering users free access, the tool supports product access via S3 resources by default, configurable through environment variables. All the above characterizes eometadatatool as the most powerful stactool (a high-level command-line tool and Python library for working with STAC) package available, providing both valid STAC items and a method for uploading them to the selected backend. 

The standard specification itself has been influenced by the CDSE catalog development process, which contributed to the evolution of the standard by introducing version 1.1 and updated extensions (storage, eo, proj) that better meet user needs. The paper discusses the most significant modifications, their impact on the catalog’s functionality, and outlines the main differences. 

Particular attention is given to performance optimization due to the substantial data volume and high update frequency. The study examines the configuration and performance testing (using Locust) of the frontend layer (stac-fastapi-pgstac) and backend (pgstac). The stac-fastapi-pgstac implementation was deployed on a scalable Kubernetes cluster and underwent a product hydration process (specific to managing JSON data in pgstac), leveraging Python's native capabilities for this task. The pgstac schema was deployed on a dedicated bare-metal server with a PostgreSQL database, utilizing master-worker replication enabled through appropriate pgstac configuration. Both software tools are open source, and the achieved optimal configurations are documented and will be presented in detail. 

The presented solution empowers the community to fully utilize the new catalog, leverage its functionalities, and access open tools that enable independent construction of STAC catalogs compliant with ESA and community recommendations. 

How to cite: Niemyjski, M. and Musiał, J.: Building the Copernicus Data Space Ecosystem STAC Catalog: Methodologies, Optimizations, and Community Impact, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17171, https://doi.org/10.5194/egusphere-egu25-17171, 2025.

EGU25-17172 | ECS | Orals | ESSI2.13

Neural Embedding Compression for Earth Observation Data – an Ablation Study 

Amelie Koch, Isabelle Wittmann, Carlos Gomez, Rikard Vinge, Michael Marszalek, Conrad Albrecht, and Thomas Brunschwiler

The exponential growth of Earth Observation data presents challenges in storage, transfer, and processing across fields such as climate modeling, disaster response, and agricultural monitoring. Efficient compression algorithms—either lossless or lossy—are critical to reducing storage demands while preserving data utility for specific applications. Conventional methods, such as JPEG and WebP, rely on hand-crafted base functions and are widely used. However, Neural Compression, a data-driven approach leveraging deep neural networks, has demonstrated superior performance by generating embeddings suitable for high levels of entropy encoding, enabling more accurate reconstructions at significantly lower bit rates.

In our prior work, we developed a Neural Compression pipeline utilizing a masked auto-encoder, embedding quantization, and an entropy encoder tailored for satellite imagery [1]. Instead of reconstructing original images, we evaluated the reconstructed embeddings for downstream tasks such as image classification and semantic segmentation. In this study, we conducted an ablation analysis to quantify the contributions of individual pipeline components—encoder, quantizer, and entropy encoder—toward the overall compression rate. Our findings reveal that satellite images achieve higher compression rates compared to ImageNet samples due to their lower entropy. Furthermore, we demonstrate the advantages of learned entropy models over hand-crafted alternatives, achieving better compression rates, particularly for datasets with seasonal or geospatial coherence. Based on these insights, we provide a list of recommendations for optimizing Neural Compression pipelines to enhance their performance and efficiency.

This work was conducted under the Embed2Scale project, supported by the Swiss State Secretariat for Education, Research and Innovation (SERI contract no. 24.00116) and the European Union (Horizon Europe contract no. 101131841).

[1] C. Gomes and T. Brunschwiler, “Neural Embedding Compression for Efficient Multi-Task Earth Observation Modelling,” IGARSS 2024, Athens, Greece, 2024, pp. 8268-8273, doi: 10.1109/IGARSS53475.2024.10642535.

How to cite: Koch, A., Wittmann, I., Gomez, C., Vinge, R., Marszalek, M., Albrecht, C., and Brunschwiler, T.: Neural Embedding Compression for Earth Observation Data – an Ablation Study, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17172, https://doi.org/10.5194/egusphere-egu25-17172, 2025.

EGU25-17326 | Orals | ESSI2.13

The UK EO DataHub - a pathfinder programme to develop a data space for UK industry, public and academic sectors 

Philip Kershaw, Rhys Evans, Fede Moscato, Dave Poulter, Alex Manning, Jen Bulpett, Ed Williamson, John Remedios, Alastair Graham, Daniel Tipping, and Piotr Zaborowski

The EO DataHub is a new national data space which has been under development as part of a two-year pathfinder programme to facilitate the greater exploitation of EO data for UK industry, public sector and academia. The project has been led by the UK National Centre for Earth Observation partnered with public sector bodies, the UK Space Agency, Met Office, Satellite Applications Catapult and National Physical Laboratory and enlisting commercial suppliers for the development and delivery of the software.

The Hub joins a crowded space in this sector as it joins a growing number of similar such platforms. However, as a national platform (with government as an anchor tenant) it is seeking to provide a unique offering as a trusted source of data, integrating curated data products from the science community building on UK strengths in climate research.

The architecture can be considered as a three layer model. At the base layer, different data sources are integrated - both commercial (Airbus and Planet Labs) and academic providers - from the CEDA data archive (https://archive.ceda.ac.uk) hosted on the JASMIN supercomputer (https://jasmin.ac.uk). The data catalogue now includes high and very high resolution SAR and optical products, Sentinel, UK Climate Projections, CMIP (https://wcrp-cmip.org), CORDEX (https://cordex.org) and outputs from EOCIS (https://eocis.org) consisting of a range of satellite-derived climate data products.

The middle layer, the Hub Platform provides services and APIs including federated search which integrates the data from the various providers, image visualisation, a workflow engine, user workspaces and interactive analysis environments. These build on the work of ESA's EOEPCA (https://eoepca.org) and apply open standards from the Open Geospatial Consortium and STAC (https://stacspec.org/) for cataloguing. In providing this suite of services, the goal is to provide a toolkit to facilitate application developers and EO specialists in building new applications and tools to exploit the data. This forms the final layer in the architecture: as part of the programme, three example application scenarios have been funded, each partnered with a target set of users. These include 1) an application taking climate projections and land surface temperature datasets to provide risk assessments for land assets (led by SparkGeo); 2) a land cover application (Spyrosoft) and finally 3), rather than an application in its own right, a project to develop a client toolkit for use with Jupyter Notebooks and a plugin integrating the Hub’s functionality into the open source GIS desktop application QGIS (work led by Oxidian).

Over the course of the programme, running in parallel to the system development, a dedicated study has been undertaken to develop a model for future sustainability of the platform tackling engagement with potential users and cost models. At the beginning, a funding call seeded early pilots to investigate application scenarios that the platform could support. As this initial phase of the Hub completes, work is underway to engage with early adopters and provide training resources for new users.

How to cite: Kershaw, P., Evans, R., Moscato, F., Poulter, D., Manning, A., Bulpett, J., Williamson, E., Remedios, J., Graham, A., Tipping, D., and Zaborowski, P.: The UK EO DataHub - a pathfinder programme to develop a data space for UK industry, public and academic sectors, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17326, https://doi.org/10.5194/egusphere-egu25-17326, 2025.

EGU25-17799 | Posters on site | ESSI2.13

Data Spaces and geodata workflows for environmental protection 

Matthes Rieke, Benjamin Proß, Simon Jikra, Sotiris Aspragkathos, Iasonas Sotiropoulos, Stamatia Rizou, and Lisa Pourcher

The concept of Data Spaces has gained traction in recent years. Major representatives emerged which have the technological maturity as well as support by relevant decision and policy makers (e.g.  the International Data Spaces Association (IDSA) or Gaia-X). These follow different architectural approaches. In this session we want to illustrate the challenges of integrating the Data Space architectures with established concepts of Spatial Data Infrastructure.

During the next 4 years, the ENFORCE project (Empower citizeNs to join Forces with public authORities in proteCting the Environment) is dedicated to fostering sustainable practices and ensuring environmental regulatory compliance by integrating citizen science with innovative technologies. By employing Living Labs and citizen science methodologies, ENFORCE will create innovative tools that bridge the gap between data reporting, monitoring, and policy enforcement. The project integrates data collection (e.g. Copernicus satellite data), analysis, and stakeholder participation to meet these goals. ENFORCE will leverage geospatial intelligence and explainable AI to enhance environmental governance. These tools and strategies will be tested and refined at eight pilot sites in seven countries, supplemented by capacity-building and policy recommendation efforts.

The design and development of a geospatial information infrastructure that supports the envisioned data workflows is a key challenge addressed by ENFORCE. This infrastructure will prioritize the integration of OGC API-driven systems into the Data Space ecosystem, forming a central component of the project’s agenda. Through development of a blueprint architecture for integration, the project will identify gaps and missing components in current systems, aligning with standards such as the FAIR principles and open data. The concepts will be facilitated in an ENFORCE “Tools Plaza”, an innovative platform providing data science and analytical capabilities for environmental compliance workflows.

How to cite: Rieke, M., Proß, B., Jikra, S., Aspragkathos, S., Sotiropoulos, I., Rizou, S., and Pourcher, L.: Data Spaces and geodata workflows for environmental protection, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17799, https://doi.org/10.5194/egusphere-egu25-17799, 2025.

EGU25-19418 | Posters on site | ESSI2.13

Lossy Data Compression Exploration in an Online Laboratory and the Link to HPC Design Decisions 

Karsten Peters-von Gehlen, Juniper Tyree, Sara Faghih-Naini, Peter Dueben, Jannek Squar, and Anna Fuchs

It is apparent that the data amounts expected to be generated by current and upcoming Earth System Science research and operational activities stress the capabilities of HPC and associated data infrastructures. Individual research projects focusing on running global Earth System Models (ESMs) at spatial resolution of 5km or less can easily occupy several petabytes on disk. With multiple of such projects running on a single HPC infrastructure, the challenge of storing the data alone becomes apparent. Further, community-driven activities like model intercomparison projects – which are conducted for both conventional and high-resolution model setups – add to the aforementioned strain on storage systems. Hence, when planning for next-generation HPC systems, the storage requirements of state-of-the-art ESM-centered projects have to be clear so that systems are still fit-for-use 5 years down the road from the initial planning stage.

As computational hardware costs per performance unit (FLOP or Byte) are not decreasing anymore like they have in the past decades, HPC system key figures do not increase substantially anymore from one generation to the next. The mismatch between demands of research and what future systems can offer is therefore clear.

One apparent solution to this problem is to simply reduce the amount of data from ESM simulations stored on a system. Data compression is one candidate to achieve this. Current ESM projects already utilize application-side lossless compression techniques, which help reduce storage space. However, decompression may incur performance penalties, especially when read patterns misalign with the compression block sizes. Lossy compression offers the potential for higher compression rates, without access penalties for data retrieval. However, its suitability is highly content-dependent, raising questions about which lossy compression methods are best suited for specific datasets. On a large scale, applying lossy compression also prompts the consideration of how such data reduction could shape the design of next-generation HPC architectures.

With lossy compression not being very popular in the ESM-community so far, we present a key development of the ongoing ESiWACE3 project: an openly accessible Jupyter-based online laboratory for testing lossy compression techniques on ESM output datasets. This online tool currently comes with a set of notebooks allowing users to objectively evaluate the impact lossy compression has on analyses performed on the compressed compared to the input data. With some compressors promising compression ratios of 10x-1000x, providing such tools to ensure compression quality is essential. The motivation behind the online compression laboratory is to foster the acceptance of lossy compression techniques by conveying first-hand experience and immediate feedback of benefits or drawbacks of applying lossy compression algorithms. 

Going one step further, we illustrate the impacts that applying lossy-compression techniques on ESM data on large-scales can have on the design decisions made for upcoming HPC infrastructures. We illustrate, among others, that increased acceptance and application of lossy compression techniques enables more efficient resource utilization and allows for smarter reinvestment of funds saved from reduced storage demands, potentially leading to the acquisition of smaller systems and thus enabling increased research output per resource used.

How to cite: Peters-von Gehlen, K., Tyree, J., Faghih-Naini, S., Dueben, P., Squar, J., and Fuchs, A.: Lossy Data Compression Exploration in an Online Laboratory and the Link to HPC Design Decisions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19418, https://doi.org/10.5194/egusphere-egu25-19418, 2025.

EGU25-20188 | ECS | Posters on site | ESSI2.13

Creating TROPOMI superobservations for data assimilation and model evaluation 

Pieter Rijsdijk, Henk Eskes, Kazuyuki Miyazaki, Takashi Sekiya, and Sander Houweling

Satellite observations of tropospheric trace gases and aerosols are evolving rapidly. Recently launched instruments provide increasingly higher spatial resolutions with footprint diameters in the range of 2–8 km, with daily global coverage for polar orbiting satellites or hourly observations from geostationary orbit. Often the modelling system has a lower spatial resolution than the satellites used, with a model grid size in the range of 10–100 km. When the resolution mismatch is not properly bridged, the final analysis based on the satellite data may be degraded. Superobservations are averages of individual observations matching the resolution of the model and are functional to reduce the data load on the assimilation system. In this paper, we discuss the construction of superobservations, their kernels and uncertainty estimates. The methodology is applied to nitrogen dioxide tropospheric column measurements of the TROPOMI instrument on the Sentinel-5P satellite. In particular, the construction of realistic uncertainties for the superobservations is non-trivial and crucial to obtaining close to optimal data assimilation results. We present a detailed methodology to account for the representativity error when satellite observations are missing due to e.g. cloudiness. Furthermore, we account for systematic errors in the retrievals leading to error correlations between nearby individual observations contributing to one superobservation. Correlation information is typically missing in the retrieval products where an error estimate is provided for individual observations. The various contributions to the uncertainty are analysed: from the spectral fitting, the estimate of the stratospheric contribution to the column and the air-mass factor. The method is applied to TROPOMI data but can be generalised to other trace gases such as HCHO, CO, SO2 and other instruments such as OMI, GEMS and TEMPO. The superobservations and uncertainties are tested in the ensemble Kalman filter chemical data assimilation system developed by JAMSTEC. These are shown to improve forecasts compared to thinning or compared to assuming fully correlated or uncorrelated uncertainties within the superobservation. The use of realistic superobservations within model comparisons and data assimilation in this way aids the quantification of air pollution distributions, emissions and their impact on climate.

How to cite: Rijsdijk, P., Eskes, H., Miyazaki, K., Sekiya, T., and Houweling, S.: Creating TROPOMI superobservations for data assimilation and model evaluation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20188, https://doi.org/10.5194/egusphere-egu25-20188, 2025.

EGU25-20430 | Orals | ESSI2.13

Compression and Aggregation: a CF data model approach 

David Hassell, Sadie Bartholomew, Bryan Lawrence, and Daniel Westwood

The CF (Climate and Forecast) metadata conventions for netCDF datasets describe means of "compression-by-convention", i.e. methods for compressing and decompressing data according to algorithms that are fully described within the conventions themselves. These algorithms, which can be lossless or lossy, are not applicable to arbitrary data, rather the data have to exhibit certain characteristics to make the compression worthwhile, or even possible.

Aggregation, available in CF-1.13, provides the utility of being able to view, as a single entity, a dataset that has been partitioned across multiple other independent datasets on disk, whilst taking up very little extra space on disk since the aggregation dataset contains no copies of the data in each component dataset. Aggregation can facilitate a range of activities such as data analysis, by avoiding the computational expense of deriving the aggregation at the time of analysis; archive curation, by acting as a metadata-rich archive index; and the post-processing of model simulation outputs, by spanning multiple datasets written at run time that together constitute a more cohesive and useful product. CF aggregation currently has cf-python and xarray implementations.

The conceptual CF data model does not recognise compression nor aggregation, choosing to view all CF datasets as if they were uncompressed and containing all of their own data. As a result, the cf-python data analysis library, that is built exactly on the CF data model, also presents datasets lazily to the user in this manner, without decompressing or re-combining the data in memory until the user actually accesses the data, at which time it occurs automatically. This approach allows the user to interact with their data in an intuitive and efficient manner; and also removes the need for the user to have to assimilate large parts of the CF conventions and having to create their own code for dealing with the compression and aggregation algorithms.

We will introduce compression by ragged arrays (as used by Discrete Sampling Geometry features, such as timeseries and trajectories) and dataset aggregation, with cf-python examples to demonstrate the ease of use that arises from using the CF data model interpretation of the data.

How to cite: Hassell, D., Bartholomew, S., Lawrence, B., and Westwood, D.: Compression and Aggregation: a CF data model approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20430, https://doi.org/10.5194/egusphere-egu25-20430, 2025.

EGU25-3945 | ECS | Posters on site | G2.6

Transforming coastal GNSS stations into tsunami gauges with GNSS-IR 

Haishan Chai, Kejie Chen, and Jian Lin

Although Global Navigation Satellite System Interferometric Reflectometry (GNSS-IR) has been extensively utilized for monitoring water levels in various bodies of water such as lakes, rivers, tides, and storm surges, its capability in detecting high-dynamic phenomena like tsunamis is still largely unexplored. This research introduces a near-real-time GNSS-IR tsunami monitoring framework, which concurrently inverses sea level, vertical sea-level velocity, and acceleration with the employment of an adaptive window strategy. Through this framework, we observed the tsunami wave of 2020 Tonga tsunami based on GNSS observations alone, with correlation of 62.9% compared with tide gauge, showing that GNSS-IR can detect tsunami waves with an amplitude of ~0.5 meters and a period of ~40 minutes. Additionally, it is discovered that the observation conditions necessary for tsunami monitoring are more stringent compared to those for tidal measurements, with a minimum requirement of six available satellite arcs (half rising and half setting) within a one-hour window. Consequently, out of 84 GNSS sites evaluated along the Pacific Rim, 29 are identified as being capable of conducting effective tsunami monitoring, whereas the remaining sites are only suitable for observing tides and storm surges.

How to cite: Chai, H., Chen, K., and Lin, J.: Transforming coastal GNSS stations into tsunami gauges with GNSS-IR, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3945, https://doi.org/10.5194/egusphere-egu25-3945, 2025.

EGU25-6360 | Posters on site | G2.6

GNSS-IR near real-time sea level retrieval from multi-constellation shared-frequency signals 

Angel Martin-Furones and Shengnan Liu

Sea level monitoring is of great significance for studying global climate change, disaster monitoring, and water resource management. GNSS Interferometric Reflectometry (GNSS-IR) technology is considered an effective complement to traditional sea level monitoring methods and has gained significant attention in recent years. However, in the two main GNSS-IR methods for sea level retrieval (spectral analysis and inverse modeling), real-time performance is limited because each low-elevation angle trajectory corresponds to a single retrieval value, and post-processing is required to eliminate outliers. In this study, we propose a near-real-time sea-level retrieval method based on shared-frequency signals. A sliding time window was used, and different strategies were employed to combine dSNRs from various satellites within the time window using both spectral analysis and inverse modeling processing methods to accurately extract the reflector height, which was further converted into sea level. Through experiments conducted at two PBO stations, we verified that near-real-time spectral analysis and inverse modeling methods can stably output sea-level retrievals within 20/30-minute time windows. Subsequently, a comparison with the traditional method revealed that the near-real-time approach enables sea-level monitoring with higher accuracy and much more uniform time resolution. This study shows that GNSS-IR technology can achieve near real-time, high-precision sea-level monitoring in multi-system scenarios and further promotes its application in sea-level monitoring.

How to cite: Martin-Furones, A. and Liu, S.: GNSS-IR near real-time sea level retrieval from multi-constellation shared-frequency signals, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6360, https://doi.org/10.5194/egusphere-egu25-6360, 2025.

EGU25-8297 | ECS | Posters on site | G2.6 | Highlight

MAGIC-CH: Machine Learning-based Advancement and Usability Assessment of GNSS Interferometric Reflectometry for Climatological Studies in Switzerland 

Laura Crocetti and Matthias Aichinger-Rosenberger

The MAGIC-CH project aims to advance the application of environmental products for climatological monitoring derived from observations of Global Navigation Satellite Systems (GNSS) Interferometric Reflectometry (IR). The project explores the potential of the existing Swiss GNSS infrastructure for monitoring essential climate variables, including snow, soil moisture, and atmospheric water vapor.

In this contribution, we aim to apply machine learning techniques to directly retrieve soil moisture and snow heights from GNSS-IR observables. Time series of signal-to-noise ratio (SNR) from ground-reflected GNSS signals are utilized as features, while satellite-based soil moisture data and in-situ snow height observations serve as target variables. Additionally, azimuth and elevation angle, day of the year, and a digital elevation model are used as inputs in the machine learning framework.

Preliminary results for soil moisture retrieval are based on the XGBoost algorithm, using GNSS data from the Automated GNSS Network for Switzerland (AGNES) and the 1 km surface soil moisture product provided by the Copernicus Global Land Monitoring Service. For snow height, initial results are based on an artificial neural network, GNSS-IR measurements of the Plate Boundary Observatory, and snow height observations of SNOTEL sites. The performance of these machine learning models shows promising improvements, significantly reducing standard error measures compared to traditional retrieval methods.

How to cite: Crocetti, L. and Aichinger-Rosenberger, M.: MAGIC-CH: Machine Learning-based Advancement and Usability Assessment of GNSS Interferometric Reflectometry for Climatological Studies in Switzerland, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8297, https://doi.org/10.5194/egusphere-egu25-8297, 2025.

EGU25-8758 | ECS | Posters on site | G2.6

Continuous coastal sea level measurement in the global geodetic coordinate frame: A realization with GNSS 

Feng Peng, Rüdiger Haas, and Gunnar Elgered

Sea level is a critical environmental parameter with significant implications for both daily life and global environmental processes. Traditionally, coastal sea levels have been measured using tide gauges. However, tide gauge measurements are affected by the vertical land motion and some sites lack a consistent reference datum on a global scale. GNSS Interferometric Reflectometry (GNSS-IR) offers a promising alternative for continuous coastal sea level monitoring within a geodetic reference frame, supporting sea level studies on a global scale. Despite its potential, GNSS-IR is hindered by various error sources that can degrade and bias sea level measurements. Achieving both precise positioning and accurate sea level monitoring simultaneously remains a significant challenge. To enhance the accuracy of GNSS-IR sea level measurements and align the results within a geodetic reference frame, we developed a dual-antenna GNSS reflectometry and positioning system. The system features a zenith-pointing GNSS antenna optimized for positioning and a horizon-pointing antenna designed for sea level monitoring. These two antennas are tightly connected, with precise measurements of the vertical distance between them. Advanced GNSS-IR error models, including antenna phase center corrections, are incorporated to mitigate errors in the sea level retrievals. The performance of this system was evaluated using nearby geodetic GNSS installations, traditional tide gauge measurements, and leveling surveys. Initial results demonstrate that the zenith-pointing antenna achieves sub-centimeter level positioning precision, comparable to nearby GNSS reference stations. The horizon-pointing antenna provides sea level measurements with an 1σ error of approximately 2 cm on a temporal resolution of 15 min. Notably, the zenith-pointing antenna performs significantly worse for sea level retrieval, while the horizon-pointing antenna is less accurate for precise positioning. These findings highlight the necessity of a dual-antenna system for achieving optimal performance in both positioning and sea level retrieval. The developed system enables continuous coastal sea level monitoring within the GNSS reference frame with centimeter-level accuracy, offering a valuable dataset contributing to global sea level studies.

How to cite: Peng, F., Haas, R., and Elgered, G.: Continuous coastal sea level measurement in the global geodetic coordinate frame: A realization with GNSS, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8758, https://doi.org/10.5194/egusphere-egu25-8758, 2025.

EGU25-16400 | Posters on site | G2.6

Sea Level estimations based on GNSS-IR with two antennas 

Nazi Wang, Fan Gao, Tianhe Xu, Xinyue Meng, Yunqiao He, and Meijun Wang

Sea level estimations have an important influence on climate research, marine transportation, production and life of coastal people and so on. Global Navigation Satellite System Interferometry Reflectometry (GNSS-IR) has been verified as a promising alternative of remote sensing technique for coastal sea level monitoring. Signal-to-noise ratio (SNR) data received by one off-shelf antenna and a classic GNSS geodetic receiver, which contain the multipath information of the station environment, were usually used for sea level retrieval. However, due to its use of only observations at low satellite elevation angles, this GNSS-IR technique is limited by its low sampling rate, for which only one sea level retrieval can be obtained for each independent satellite ascending or descending arc. In this study, we proposed to use an improved GNSS-IR setup with two antennae to improve the sampling rate by realizing sea level estimation from both high- and low- elevation angle observation. Compared to the traditional GNSS station with one upward right-hand circular polarized (RHCP) antenna and one geodetic receiver, this new setup added one downward left-hand circular polarized (LHCP) antenna and one combiner.  Observations of the two antennae combined by the combiner were input to the geodetic receiver to output RINEX files. SNR data from the RINEX files were then used to estimate sea level. One-month coastal experiment using the new setup was performed from January 4, 2023, to February 5, 2023, in Weihai, China. By comparing with co-located tide gauge data, sea level estimations with RMSE of 7 cm and correlation coefficient of 0.99 were obtained from the experimental data obtained by using the proposed setup. Moreover, the results showed that, by using the proposed GNSS-IR setup, the sampling rate of sea level estimations was improved about 3 times comparing to the results of conventional setup with one antenna. Because of the cheap price of LHCP antenna and combiner, the proposed GNSS-MR setup can improve its sampling rate of retrievals while maintaining its low-cost advantage. This new setup could be applied to other GNSS-IR sites and is therefore beneficial for global sea level monitoring.

How to cite: Wang, N., Gao, F., Xu, T., Meng, X., He, Y., and Wang, M.: Sea Level estimations based on GNSS-IR with two antennas, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16400, https://doi.org/10.5194/egusphere-egu25-16400, 2025.

EGU25-17647 | ECS | Posters on site | G2.6

Performance of Raspberry Pi Reflectors and multiple in-situ sensors for surface water monitoring and sentinel-3 validation over two years 

Makan Karegar, Jiaming Chen, Luciana Fenoglio-Marc, and Jürgen Kusche

As part of the Collaborative Research Center (SFB 1502) funded by the German Research Foundation (DFG), a project is being carried out to analyze surface water levels and discharge using data from the latest generation of satellite altimetry. Within this project, a network of eight Raspberry Pi Reflectors (RPR) (Karegar et al. 2022, WRR) was strategically installed in the middle Rhine valley and upper Rhine along a stretch of about 110 km during the spring and summer of 2023. While the primary goal of this deployment was to validate SWOT (Surface Water and Ocean Topography) surface water level observations, four RPRs were also placed under Sentinel-3 tracks A156 and B156. Sentinel-3 L1A data were acquired and processed using the Fully Focused SAR (FFSAR) processor and automatic off-nadir processing method (Chen et al. 2025, J. Hydrology). At Worms, multiple in-situ sensors are being used. The river gauge maintained by the German Federal Waterways and Shipping Administration (WSV) records water levels at 15-minute intervals. It is a classic float and stilling well gauge located on the riverbank and connected to the water via an underground pipe. A commercial radar sensor from Vortex-io was mounted on a bridge overlooking the river. Also, an RPR was installed in Worms to evaluate its performance. Having these three sensors based on different techniques allows us assess their consistency together with Sentinel-3 observations. This presentation particularly reports on the RPR’s behavior and long-term performance in off-grid regions where there is no grid coverage or local power supply. We will also discuss their application in validating Sentinel-3 data, especially in the steep and narrow Middle Rhine Valley where the surrounding terrain significantly influences the accuracy of both GNSS-IR and Sentinel-3 measurements.

How to cite: Karegar, M., Chen, J., Fenoglio-Marc, L., and Kusche, J.: Performance of Raspberry Pi Reflectors and multiple in-situ sensors for surface water monitoring and sentinel-3 validation over two years, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17647, https://doi.org/10.5194/egusphere-egu25-17647, 2025.

EGU25-19433 | Posters on site | G2.6

Extended Kalman filtering for high-rate GNSS-R sea level measurements : Achieving centimeter-level precision during Hurricane Milton at Cedar Key 

Aurélien Pira, Alvaro Santamaría-Gómez, and Guy Wöppelmann

Sea level monitoring is vital for applications such as urban planning and climate studies. Traditional tide gauges, which often use radar measurements, remain the most common method but require placing sensors near the water surface, exposing them to potential damage in hostile maritime environments.

The demand for precise and high-frequency sea level monitoring has led to the development of innovative techniques, including Global Navigation Satellite System Reflectometry (GNSS-R). This promising method enables continuous, global sea level measurements (e.g., Larson et al., 2013) without the limitations of traditional sensors such as underwater (pressure gauges), in contact (float gauges), or above-surface (acoustic and radar). Furthermore, it takes advantage of the high availability of existing GNSS installations around the globe, potentially expanding the scope of tide gauge measurements on a global scale.

GNSS-R measurement methods are typically based on the analyze of the Signal-to-Noise Ratio (SNR) and most of the applied methods are using spectral analysis, such as Lomb-Scargle periodograms, to achieve centimeter-level accuracy in average sea level estimation (Larson, Ray and Williams, 2017). However, these methods require long SNR time series, limiting their ability to capture high-frequency sea level variations. This as the effect to restricted spectral methods to observing slow sea level variations, such as tides. Recent advancements have demonstrated that Kalman filtering can achieve sub-5 cm accuracy while increasing data sampling rates (e.g., Santamaría-Gómez and Watson, 2017; Strandberg, Hobiger and Haas, 2019; Liu et al., 2023).

We present a novel approach to enhance the accuracy and temporal resolution of sea level observations from SNR analysis, using an Extended Kalman Filter (EKF) to estimate SNR oscillation frequency and amplitude. The main advantage it to abble to ofer a flexibility to select the sampling rate of the resulting time series, allowing sea level estimates at rates up to the original SNR measurement frequency.

Our approach integrates data from all available GNSS constellations and carriers, improving data redundancy and robustness, particularly during signal loss or satellite transitions. Additionally, we apply a correction for phase center offset (PCO) variations, specific to each carrier and antenna model. This ensures that the resulting water height time series is referenced to a precise physical point, the Antenna Reference Point (ARP).

We validated our method by reconstructing a year-long sea level time series at Brest, France, with a 10-second sampling interval. We finally achieved a root-mean-square-error (RMSE) of 2.6 cm compared to the data of a co-located radar tide gauge. Similar performance was observed at other sites, with sampling rates as high as 1 second. Furthermore, the algorithm's ability to track irregular and unpredictable sea level variations beyond tidal models was evaluated during 10 days of observation at Cedar Key (Florida, USA) during Hurricane Milton. The resulting water height time series showed an RMSE of 1.9 cm compared to the data of a co-located tide gauge, demonstrating the method's efficiency under complex hydrodynamic conditions.

How to cite: Pira, A., Santamaría-Gómez, A., and Wöppelmann, G.: Extended Kalman filtering for high-rate GNSS-R sea level measurements : Achieving centimeter-level precision during Hurricane Milton at Cedar Key, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19433, https://doi.org/10.5194/egusphere-egu25-19433, 2025.

EGU25-878 | ECS | Orals | NH8.2

Geogenic radon potential through geostatistical analysis of uranium concentration 

Linda Bonorino, Gianluca Beccaris, Paolo Chiozzi, Andrea Cogorno, Elga Filippi, Sonja Prandi, and Massimo Verdoya

Dosimetric measurements are customarily conducted in dwellings to evaluate the radon hazard. The measurement sites are often unevenly distributed. This makes challenging direct data interpolation and their extrapolation to under-sampled areas, as well as the prediction of hazard. Geostatistical techniques, such as logistic regression, help address this issue because they allow for using proxy data to infer the probability of radon hazards where no direct measurements are available. The rock U content can be an appropriate proxy for indoor 222Rn concentration. Considering uranium concentrations in combination with other variables, such as bedrock nature and surface geology, has emerged as an effective method for producing reliable maps of Geogenic Radon Potential (GRP), a hazard indicator of radon generated by the radioactive decay of elements in rocks and soils and released into the air.  In this paper, we investigated the relationship between uranium and radon to map the radiological hazard linked to lithology also in unsampled areas. We used field gamma-ray spectrometry to determine the uranium concentration on the exposed bedrock and radon dosimetric records in indoor environments in direct contact with the ground. In addition to passive radon determinations, we measured the radon in soils by means of an active device. Logistic regression was used to examine the correlation between the concentration of uranium and the indoor radon measured in the same geological formation. This technique was tested in Western Liguria (Northern Italy), an area including a wide range of rocks spanning from sedimentary and metasedimentary to metavolcanic. The approach led to determining the probability of exceeding the threshold of 200 Bq/m3 for each lithology based on U concentration and defining a detailed picture of the investigated area's GRP. A background uranium content of 4 ppm implies a 50% probability of exceeding the safety threshold of indoor radon. Although the dataset of soil radon measurements so far collected is far from being representative, the results indicate that higher concentrations (up to 250 kBq/m3 as an upper bound) roughly correspond to indoor radon > 200 Bq/m3. In summary, our work highlights the relationship between indoor radon concentration and uranium content in rocks and reinforces the use of geological data to identify areas with a higher susceptibility to radon exposure.

How to cite: Bonorino, L., Beccaris, G., Chiozzi, P., Cogorno, A., Filippi, E., Prandi, S., and Verdoya, M.: Geogenic radon potential through geostatistical analysis of uranium concentration, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-878, https://doi.org/10.5194/egusphere-egu25-878, 2025.

EGU25-1184 | Posters on site | NH8.2

A multidisciplinary monitoring approach involving radioactivity, greenhouse gas emissions, stratigraphy and rock magnetism 

Alessandra Sciarra, Mariarosaria Falanga, Simona Mancini, Michele Guida, Fausto Grassa, Valeria Misiti, Stefania Pinzi, Gianfranco Galli, Alessandra Venuti, and Antonio Cascella

Mud volcanoes (MV), classified as "sedimentary volcanism", represent the surface expression of underground processes characterized by movements of large masses of fluids (water and gas) and sediments. Some MVs can represent a serious source of geohazards, mainly related to paroxysmal events with flooding of huge amounts of mud that can damage structures and seriously injure people in their vicinity. Although MVs constitute a source of geohazard, albeit limited to their proximity, monitoring protocols for their surveillance have never been employed. Gas released from mud volcanoes consists mainly of CH4 and minor components N2, O2, CO2 and light hydrocarbons, but radon emission rate has been poorly studied. With the aim of filling this knowledge gap, the present work proposes a multidisciplinary approach to the study of MVs, with the final goal of identifying reliable indicators of their state of activity that could be used as precursors of paroxysmal events and their dangerousness for the population. The multidisciplinary monitoring method used to study the Salse di Nirano MVs is based on radioactivity and greenhouse gas emissions, stratigraphy and magnetism of the rocks in order to develop a model of the space-time evolution of their activity and identify any variations. To estimate the amount of gas released, some surveys of flux measurements (CO2, CH4) and gas content (CO2, CH4, 222Rn, 220Rn) were conducted.

Furthermore, with the aim of identifying a correlation between methane emissions and radon activity, a series of laboratory tests were performed in a controlled system.

Salse di Nirano are within a natural reserve, visited by many people every year, so the definition of the natural gas hazard estimation is essential for the protection of the population and extremely useful for the local authorities. Our objective is to acquire a better understanding of the processes happening in the eruption conduit, the activity (speed and intensity of gas migration) of the seepage system connected to the feeding reservoir, and the interaction between faults and deep and/or shallow reservoirs. The results can also be exported to other areas characterized by the presence of sedimentary volcanism.

How to cite: Sciarra, A., Falanga, M., Mancini, S., Guida, M., Grassa, F., Misiti, V., Pinzi, S., Galli, G., Venuti, A., and Cascella, A.: A multidisciplinary monitoring approach involving radioactivity, greenhouse gas emissions, stratigraphy and rock magnetism, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1184, https://doi.org/10.5194/egusphere-egu25-1184, 2025.

EGU25-1612 | Orals | NH8.2

Nuclide specific transfer of radium from soils to plants 

Jens Fohlmeister, Michaela Achatz, and Peggy Hofmann

For a comprehensive assessment of radiation exposure from naturally occurring radionuclides in soils, the ingestion pathway of foodstuffs grown on such soils may be a major contributor. Often, only measurement results of the radionuclide vector of the soil are available for an initial dose estimation. For such calculations, however, the activity concentrations in plants are crucial. These can generally be estimated from the soil data using soil-to-plant transfer factors. Typically, these transfer factors are used on an elemental basis, i.e., not specific to individual nuclides of the same element. The reason behind this approach appears to be based on limited measurement availability for several nuclides of the same element. Thus, the transfer factors have preferably been determined only for the more easily measurable nuclide of an element but mostly find application for all nuclides of this element.

However, for nuclides of an element that display significant differences in their radiotoxicity, potential but previously unconsidered radionuclide-specific differences in the soil-to-plant transfer factors can result in a significant under- or overestimation of the ingested dose. This is especially true for radium, as 228Ra causes a dose that is approximately 3 to 6 times higher than that of 226Ra. Therefore, in this contribution we will analyse the validity of equal soil-to-plant transfer factors for 226Ra and 228Ra based on a large, representative data set of a recent total diet study and data available in the literature. First results suggest that on average there is a change in the radium activity ratio during the transfer of radium between soils and plants, with 228Ra being approximately nearly twice as effectively taken up by plants compared to 226Ra.

How to cite: Fohlmeister, J., Achatz, M., and Hofmann, P.: Nuclide specific transfer of radium from soils to plants, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1612, https://doi.org/10.5194/egusphere-egu25-1612, 2025.

Atmospheric nuclear tests until 1980 and in particular the Chernobyl nuclear accident in April 1986 left considerable amounts of caesium in the environment of Eastern, Northern, and Central Europe. Regional information on the current distribution of caesium is very limited. Airborne gamma-ray spectrometry or radiometry is routinely used to investigate the regional distribution of the naturally occurring radio-elements K-40, U-238 and Th-232 in the rocks and soils of the earth’s surface and to derive compositional and geological information. Due to the large source-receiver distance and the low activity sources, large-volume scintillation detectors are used for this purpose. The spectral resolution of these instruments is low compared to laboratory setups. Therefore, the identification of photo peaks of artificial isotopes in airborne gamma-ray spectra is not straight forward and attempts to routinely determine Cs-137 signals are rare.

In this study, helicopter radiometry data that was originally collected for soil science applications in northern Germany was examined with regard to its Cs-137 information content. The spectra were acquired with a 4x4 litre NaI, 1024 channel instrument (Radiation Solutions). The overlap of the Cs-137 photo peak at 662 keV with Tl-208 and Bi-214 photo peaks from the uranium and thorium decay chains led to the development of a spectral unfolding method. In the spectra corrected in this way the intensity of the Cs-137 signal could be determined. These Cs-137 intensity values were then compared with measurements on the ground, so that a calibration of the airborne system for absolute ground activities of Cs-137 was possible. Applied to large airborne data sets covering areas in the order of 100 km2 resulted in activity maps that give interesting insights into the present day Cs-137 levels in the environment of Northern Germany.

How to cite: Ibs-von Seht, M.: Determination of environmental Cs-137 levels from standard airborne gamma-ray spectrometry data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1777, https://doi.org/10.5194/egusphere-egu25-1777, 2025.

EGU25-2764 | Posters on site | NH8.2

Addressing water security using 36Cl 

Chiara Telloli, Fabio Borgognoni, and Antonietta Rizzo

Semi-arid regions, characterized by low and erratic rainfall, need significant efforts in managing their water resources. Groundwater, a vital resource in these areas, is often overexploited, leading to depletion and degradation. The lack of suitable data and methods to quantify regional hydrological processes often requires a comprehensive understanding of groundwater systems, including their recharge rates, flow patterns, and water quality and the adaptation to climate change.

To date, groundwater management is primarily based on hydrogeological modeling and key parameters such as recharge rate and groundwater dynamics.

The use of radioisotopes makes it possible to date groundwater resources and evaluate its recharge times. By using a combination of residence time indicators (3H, 14C, 36Cl) and stable water isotopes (2H and 18O), it is possible to provide a greater constraint on the residence time of water in groundwater aquifers.

Thanks to the advancement analytical techniques on the use of 36Cl, present in the environment following nuclear tests, is a promising method for estimating water transit times and recharge rates of aquifers on a basin scale and for distinguishing water and chloride cycles.

Studies have already been carried out in the Chari-Logone aquifer of the emblematic Lake Chad basin, located in the central Sahel, where the analysis of 36Cl in the central areas shows the presence of very old groundwater (<2 Ma), suggesting that the aquifers in the Sahel host a significant amount of renewable water, which could therefore be used as a strategic freshwater resource.

Continued investment in developing reliable and less time-consuming analytical techniques is crucial to manage groundwater resources sustainably in semi-arid regions.

How to cite: Telloli, C., Borgognoni, F., and Rizzo, A.: Addressing water security using 36Cl, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2764, https://doi.org/10.5194/egusphere-egu25-2764, 2025.

EGU25-4025 | Orals | NH8.2

Application of fallout-derived 239+240Pu for estimating soil redistribution rates at an olive orchard under Mediterranean climate  

José Luis Mas, Santiago Hurtado-Bermúdez, Andrés Peñuela, Vanesa García-Gamero, Tom Vanwalleghem, and Adolfo Peña

Soil erosion significantly threatens soil health in semiarid regions such as the Mediterranean. Fallout radionuclides (FRNs), deposited from atmospheric fallout, accumulate in the soil profile and their redistribution patterns can be used to estimate soil erosion and deposition rates.  While 137Cs has been traditionally used for soil redistribution studies, this research explores the application of fallout-derived 239+240Pu in an olive orchard under Mediterranean climate conditions (Montefrío, Granada, Spain). The spatial variability of the reference profiles was assessed by replicating the sampling four times. Soil redistribution rates, estimated using the MODERN model, were compared with the inventory method for eroded sites, demonstrating excellent agreement (Pearson’s r = 0.9995, slope = 0.993 ± 0.006 t ha-1·yr-1)/(t·ha-1·yr-1)). Estimated  erosion and deposition rates ranged from 0 to -76 t ha-1 yr-1 and from 0 to +29.9 t ha-1·yr-1, respectively, indicating a significant soil degradation. These results highlight the potential of Pu isotopes as a valuable tool for assessing soil dynamics in Mediterranean agricultural systems.

How to cite: Mas, J. L., Hurtado-Bermúdez, S., Peñuela, A., García-Gamero, V., Vanwalleghem, T., and Peña, A.: Application of fallout-derived 239+240Pu for estimating soil redistribution rates at an olive orchard under Mediterranean climate , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4025, https://doi.org/10.5194/egusphere-egu25-4025, 2025.

EGU25-4150 | ECS | Orals | NH8.2

Innovative Radon Mitigation: A Long-Term Study on the Effectiveness of Decentralised Ventilation with Heat Recovery 

Diana Altendorf, Florian Berger, Jörg Dehnert, Michal Duzynski, Hannes Grünewald, Ralf Trabitzsch, and Holger Weiß

Radon-222 is a naturally occurring radioactive gas and a significant indoor air pollutant. Elevated indoor radon activity concentration significantly increases this risk of lung cancer for individuals. In accordance with the European Euratom Directive, the German government has established a reference value of 300 Bq/m³ as the annual mean for radon activity concentration in indoor workplaces and living spaces. Mitigating indoor radon is essential to ensure healthy living and working environments, particularly in areas with heightened radon exposure. This study presents the results of a three-year proof-of-concept investigation into the effectiveness of a decentralised ventilation system with heat recovery as a radon mitigation strategy.

Therefore, a series of ventilation experiments were performed in an unoccupied ground-floor flat of a residential building in Aue-Bad Schlema, Germany. Located within one of Saxony’s radon-prone areas in the Ore Mountains (Erzgebirge), a region well-known for its numerous ore deposits and an 800-year long mining history. The flat was divided into three individually controllable ventilation zones using strategically positioned ventilation devices with heat recovery (inVENTer GmbH, Germany). These devices were controlled by a real-time measurement of indoor radon activity concentration (Smart Radon Sensors by SARAD GmbH, Germany), enabling dynamic and responsive operation of the ventilation system. By using the actual measured radon concentration [Rn] as a control parameter, the system can automatically switch between three distinct ventilation modes - "Heat Recovery", "Cross-Ventilation" and "Differential Pressure" - or deactivate entirely. Within each mode, both airflow direction and air volume flow rates can be adjusted, providing tailored solutions for effective radon mitigation.

Overall, the decentralised ventilation system with heat recovery demonstrated significant potential for reducing indoor radon concentration, achieving reductions of up to 80 %. The effectiveness of the system varied based on factors such as initial room-specific radon levels, fan performance settings, and meteorological parameters like outdoor temperature and wind speed. The study also evaluated the dependencies between indoor radon levels and various environmental and site-specific factors. Results revealed that radon dynamics are influenced by a complex interplay of geological, meteorological and building-specific characteristics - including structural design and ventilation system configuration. Different ventilation modes, combined with varying fan performance levels, contributed to distinct radon reduction outcomes, highlighting the importance of customising mitigation strategies.

These findings emphasize the necessity of integrating environmental and building-specific considerations into radon risk assessment and mitigation planning. Customised, site-specific radon mitigation strategies are essential to account for the variability introduced by local conditions, ultimately improving indoor air quality and reducing health risks in radon-affected regions.

How to cite: Altendorf, D., Berger, F., Dehnert, J., Duzynski, M., Grünewald, H., Trabitzsch, R., and Weiß, H.: Innovative Radon Mitigation: A Long-Term Study on the Effectiveness of Decentralised Ventilation with Heat Recovery, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4150, https://doi.org/10.5194/egusphere-egu25-4150, 2025.

EGU25-4205 | Posters on site | NH8.2

Radiation protection aspects in conjunction with re-use of residues from the geoenergy industry 

Tatiana Goldberg, Nicole Klasen, Simona Regenspurg, and Patrick Frings

The trend towards increasing circular economy calls for re-use of all types of waste, including recycling from industrial residues such as NORM (Naturally Occurring Radioactive Materials). These secondary raw materials are currently being considered and partly used in construction materials, for critical element extraction, in medicine, and in carbon sequestration. In the geothermal, oil and gas industry mineral deposits (scales) form during deep fluid production due to changes in thermodynamic conditions and may incorporate significant amounts of natural radionuclides. Currently these residues are discarded although the scales may contain valuable metals.

Scale samples were collected from the well and aboveground geothermal facilities and analysed via XRD, XRF and ICP-MS. Their main mineralogical constituents range from Sr-rich barite, laurionite, native copper, sulphide minerals to magnetite. Some scales contain economically viable elements, such as Cu, Ba, As and Zn. Rare earth elements also occur in minor amounts (∑ ~ 50 ppm). Radionuclide activities on bulk samples were measured via gamma-spectrometry and vary from below 1 Bq/g up to 130 Bq/g, 57 Bq/g, 63 Bq/g and 40 Bq/g for Ra-226, Pb-210, Ra-228 and Th-228, respectively. Thus, for some samples the measured activities fall within the category of surveillance.

The association between mineralogy and radionuclides is investigated following partial leaching and sequential extraction. Kind and activity concentrations of radionuclides depend on the extraction method, which is determined by the mineral phase of the targeted element. The extraction process will require dose measurements followed by a calculation of the exposure to ionizing radiation. This evaluation represents a preliminary study towards the usability of the scales and demonstrates the need for further research on recycling of the residues, with due consideration given to radiation protection aspects. 

How to cite: Goldberg, T., Klasen, N., Regenspurg, S., and Frings, P.: Radiation protection aspects in conjunction with re-use of residues from the geoenergy industry, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4205, https://doi.org/10.5194/egusphere-egu25-4205, 2025.

EGU25-8454 | ECS | Posters on site | NH8.2 | Highlight

RockyRAD: a hands-on kit for exploring rock radioactivity 

Matteo Albéri, Maria Annunziata, Pierluigi Barba, Alessio Barbagli, Enrico Chiarelli, Tommaso Colonna, Alessandro Cortopassi, Nedime Irem Elek, Fabio Gallorini, Jacopo Givoletti, Enrico Guastaldi, Fabio Mantovani, Cristina Mattone, Massimo Morichi, Dario Petrone, Silvio Pierini, Claudio Raffo, Kassandra Giulia Cristina Raptis, Virginia Strati, and Franco Vivaldi

RockyRAD represents an evolution of the traditional Geiger counter, transforming it into a complete and innovative educational tool. This compact and portable device is part of a kit containing rock samples, selected for their varying levels of natural radioactivity. These samples allow students to investigate the radioactivity of rocks, understanding how it is influenced by internal factors such as chemical composition, rather than external characteristics such as color or texture.

Students can compare the radiation levels of igneous and sedimentary rocks, assess the effectiveness of shielding materials, or conduct long-term background radiation measurements. This hands-on approach provides a deeper understanding of the radioactivity originating from natural radioisotopes (e.g., U-238) and their decay products as well as the interactions between radiation and matter.

Through an Android app, users can share results, export data for analysis, and plan extended experiments, making it suitable for citizen science. Students can evaluate reliability, calculate uncertainties, and observe how these change with measurement time, linking experimental observations to theoretical principles. The device provides both counts per minute (CPM) and equivalent dose rate (nSv/h), facilitating the understanding of absorbed dose concepts.

Teachers can design experiments tailored to school curricula, fostering an interdisciplinary approach that integrates physics, Earth science, and statistics.

In today’s energy landscape, where nuclear power is regaining attention, RockyRAD promotes scientific inquiry and awareness. By studying rock radioactivity, students develop a deeper understanding of environmental radiation, supporting informed perspectives on nuclear energy and other energy choices.

How to cite: Albéri, M., Annunziata, M., Barba, P., Barbagli, A., Chiarelli, E., Colonna, T., Cortopassi, A., Elek, N. I., Gallorini, F., Givoletti, J., Guastaldi, E., Mantovani, F., Mattone, C., Morichi, M., Petrone, D., Pierini, S., Raffo, C., Raptis, K. G. C., Strati, V., and Vivaldi, F.: RockyRAD: a hands-on kit for exploring rock radioactivity, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8454, https://doi.org/10.5194/egusphere-egu25-8454, 2025.

EGU25-8682 | ECS | Posters on site | NH8.2

Identifying Radon hazard areas: Machine learning-driven Geogenic Radon Potential mapping in Hessen 

Augustine Maada Gbondo, Rouwen Lehne, Eric Petermann, and Andreas Henk

The health impacts of the radioactive Radon are well-documented by the World Health Organization (WHO) and numerous studies. Geogenic Radon Potential (GRP) refers to the natural production of Radon by the Earth, independent of anthropogenic influences. GRP has been a focal point of research aimed at understanding the factors influencing radon variability and its spatial distribution. However, the limited availability of systematic soil-gas radon concentration measurements, along with other constraints, often leads to coarse-resolution modeling of GRP. With the availability of adequate and quality data, regional studies can be promising in investigating these influencing factors, and modelling of GRP hazards at finer spatial scales.

 

This study uses GRP survey data provided by the Hessian Agency for Nature Conservation, Environment and Geology (HLNUG) to develop machine learning models for predicting the spatial distribution of GRP in the state of Hessen, Germany, and to produce a high-resolution GRP hazard map. The models employed include Random Forest Regressor (RF), Support Vector Regressor (SVR), Gradient Boosting Regressor (GBR), and Multi-Layer Perceptron Regressor (MLPR). The dataset comprises 1,509 GRP sampling points for an area of about 21.000 km², and 37 potential predictors related to geology, soil characteristics, and climatic variables—key factors known to influence radon levels. Sequential Feature Selection (SFS) and a 5-fold spatial cross-validation strategy were employed to mitigate autocorrelation effects and enhance model generalization. Model performance was evaluated using multiple metrics and compared against ground-truth values and local geology.

 

Results revealed that the RF and GBR models outperformed others, achieving R² scores of 0.69 and 0.65 on the validation dataset, respectively, while the SVR and MLPR models underperformed. Predicted GRP values ranged from 8.9 to 178.2 for RF and 1.7 to 268.4 for GBR. Geological and soil properties emerged as the dominant predictors of GRP variability in Hessen, with predicted maps highlighting a strong dependence on local geological features. High-risk areas were effectively identified by the RF model. The study also highlights the need for additional measurements in data-scarce regions and the exploration of hybrid physics-based models that integrate domain-specific knowledge into spatial predictions.

How to cite: Gbondo, A. M., Lehne, R., Petermann, E., and Henk, A.: Identifying Radon hazard areas: Machine learning-driven Geogenic Radon Potential mapping in Hessen, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8682, https://doi.org/10.5194/egusphere-egu25-8682, 2025.

EGU25-8873 | ECS | Posters on site | NH8.2

Radionuclides on the Move: Insights into Water-Bound Soil Transport Processes 

Marc Johnen, Dr. Katja Brennan, Salim Gülez, Dr. Andre Filby, Dr. Margarita Tzivaki, and Dr. Andreas Artmann

In Germany, radionuclide exposure is calculated for various scenarios according to derived international standards (AVV-Tätigkeiten 2020). The radiation protection law and the relevant administrative regulations (StrlSchG, StrlSchV) define exposure limits and the implementation of the calculations. These administrative regulations are used in authorisation procedures and in the prospective determination of the expected exposure of individuals in the population. These regulatory measures are intended to ensure the protection of the population from additional radioactive radiation within the framework of the 10 µSv criterion of the IAEA (IAEA 1988 Safety Guides No. 89). Understanding the underlying mechanisms of radionuclide transport in defined ecosystems is pivotal to achieve the best-estimated scenarios.

Contamination of the soil can occur through air or water discharge. Discharge via air can result in dry or wet deposition. In the case of discharge via water, contamination can occur through artificial irrigation, sediment deposition from irrigated fields or contamination of soils in floodplains. All these pathways are considered relevant for assessing radionuclide fate and transport through soil.

In the current project, the transport processes of these contamination pathways on cropland and pasture are analysed in more detail aiming to identify the driving parameters and review all processes that have not yet been included in the equations in the calculation bases. Soil properties and hydrogeological characteristics play an essential role in water-bound transport in the soil. Soils are divided into different soil horizons (O, A, B, C and R horizons) with different properties, which are subject to seasonal changes as well as changes caused by cropland use and pasture. For dissolved substances, chemical processes such as speciation and complex formation, solubility and solution kinetics, retention by sorption and redox reactions play an important role, often strongly dependent on pH values. In addition to chemical processes, physical processes such as advection, diffusion, dispersion, and capillary rise are also relevant. At the root-soil interface, biological processes such as root exudation, mycorrhizal symbiosis (fungal activity), root-hair interactions and plant-controlled water movements within the plant are increasingly important. In terms of plant species, a distinction is made between leafy vegetables, root vegetables and grains.

The aim of the work is to take an interdisciplinary and holistic look at possible contamination pathways in soils by means of a system analysis. The BIOMASS process involving the definition of a FEP (Features, Events and Processes) list and visualizing it in an interaction matrix for the analysis. This conceptual model will be used to implement the appropriate mathematical models for each interaction between compartments. The concentration in the soil will then be calculated using a compartment model or numerical groundwater models. Different methods and models will be analysed and applied in individual cases. The key challenges are the different scales of the area to be analysed, the heterogeneity of the soil and the general uncertainty in the data.

How to cite: Johnen, M., Brennan, Dr. K., Gülez, S., Filby, Dr. A., Tzivaki, Dr. M., and Artmann, Dr. A.: Radionuclides on the Move: Insights into Water-Bound Soil Transport Processes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8873, https://doi.org/10.5194/egusphere-egu25-8873, 2025.

EGU25-9446 | Posters on site | NH8.2

Environmental Radioactivity and Plants Adaptations in the Maccalube Nature Reserve (Ag): Insights and Implications for the sedimentary volcanic source 

Mariarosaria Falanga, Zahra Alizadesh, Emanuele Rosa, Nunziatina De Tommasi, Simona Mancini, Serpil Aközcan Pehlivanoğlu, and Paola Cusano

This research focuses on the Maccalube di Aragona Nature Reserve (Agrigento, Italy), studying environmental radioactivity and plant activity in the context of mud volcano dynamics. The Reserve contains several gryphons and pools emitting methane, hydrocarbons, and highly saline water. Occasionally, these volcanoes experience explosive events, such as a fatal explosion in 2014. The research is part of the Promud project- INGV (https://progetti.ingv.it/it/promud), which aims to assess the Reserve’s geophysical, seismological, geodetic, and biodiversity characteristics for civil protection purposes.

Two field surveys were conducted to measure environmental radioactivity, focusing on 222Rn and 220Rn emissions from soil gas by means of specific accessorized equipment (RAD7). The main aim was to acquire more data to support the identification of the source location in a compact clay layer. Results showed a high concentration of 222Rn only in correspondence with the active emitting centers, whereas concentrations below the instrumentation sensitivity were revealed elsewhere. Moreover, the radioactive contents were determined in muds, soils, and parts of the plants (especially leaves) taken in the surroundings. Particularly, 226Ra, 232Th, 40K, and 137Cs were measured by using gamma spectrometry. Very homogeneous concentrations of previous radionuclides were found, except for 40K measured in the dried plants suggesting a possible link between that radionuclide and the plant’s activity.

Studying plants that thrive in extreme environments could provide valuable insights into the relationship between soil properties and reservoirs. For this study, the halophytic species Suaeda vera, collected from the Maccalube Reserve, was used as a model. Samples were also collected from a mountainous habitat to compare its metabolism under stressed and stress-free conditions. An untargeted metabolomic analysis of hydroalcoholic extracts of aerial parts of S. vera, performed using HR-LC-MS, revealed a diverse and rich phytochemical profile. This analysis identified a wide range of specialized metabolites. Plants from the Maccalube region have an interesting phytochemical profile, producing sulphated metabolites, particularly flavonoids, which are rare and often associated with survival in harsh environments. This secondary metabolism suggests a local biochemical adaptation of the Maccalube population. It may be influenced by the harsh environmental conditions of the region.

How to cite: Falanga, M., Alizadesh, Z., Rosa, E., De Tommasi, N., Mancini, S., Aközcan Pehlivanoğlu, S., and Cusano, P.: Environmental Radioactivity and Plants Adaptations in the Maccalube Nature Reserve (Ag): Insights and Implications for the sedimentary volcanic source, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9446, https://doi.org/10.5194/egusphere-egu25-9446, 2025.

EGU25-11146 | Posters on site | NH8.2

The Italian radon risk map 

Giancarlo Ciotoli, Eleonora Benà, Federico Mori, Livio Ruggiero, Stan Eugene Beaubien, Alessandra Sciarra, Monia Procesi, Claudio Mazzoli, Raffaele Sassi, and Sabina Bigi

Radon (²²Rn) is a naturally occurring radioactive gas that occurs in rocks and soils, and its migration pathways are influenced by geological faults. These processes can significantly increase radon leakage into buildings, posing a significant health risk. Classified as a carcinogen by the World Health Organisation, exposure to radon has required the establishment of national reference levels across Europe under Directive 2013/59/EURATOM and the identification of Radon Priority Areas (RPAs) to guide remediation initiatives. This legislation emphasises the need for both collective and individual risk management, using advanced radon risk assessment tools.

In this study, we present an innovative approach to construct a geogenic radon hazard index (GRHI) map for Italy using a robust bottom-up methodology. Our approach integrates several geological proxies related to radon source (e.g. geology, radionuclide content) and migration pathways (e.g. faults) using supervised auto-machine learning (Autogluon). A dataset of approximately 30,000 soil radon measurements was divided into training and test datasets. A conceptual model with ten predictors was developed to estimate soil radon concentrations at unsampled locations on a 1x1 km grid. The LightGBMLarge algorithm resulted in the best model (R²test = 0.524) which was validated by a combination of statistical metrics. The SHAP analysis highlighted the relative importance of the predictors in the model.

The GRHI map was further combined with census section data (ISTAT database) and population density to produce a risk map from Collective Risk Areas (CRA) to Individual Risk Areas (IRA). This final map serves as a valuable tool for national and regional administrations to identify IRAs in accordance with Directive 2013/59/EURATOM (Article 103).

This research addresses the lack of a standardised European methodology for radon risk assessment. It provides a comprehensive framework to bridge the gap between collective and individual risk. Through the integration of geological knowledge with machine learning and demographic data, this work provides useful information for the improvement of radiation protection and public health strategies.

How to cite: Ciotoli, G., Benà, E., Mori, F., Ruggiero, L., Beaubien, S. E., Sciarra, A., Procesi, M., Mazzoli, C., Sassi, R., and Bigi, S.: The Italian radon risk map, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11146, https://doi.org/10.5194/egusphere-egu25-11146, 2025.

EGU25-13183 | Orals | NH8.2

Development of an active alpha particle detector for radon measurements 

Tóth Szabolcs, Horváth Ákos, and Máthé Kálmán

In connection with the recultivation and environmental monitoring activities of the Mecsek uranium ore mine closure, several deep boreholes have been drilled. These deep boreholes are suitable for investigating spatial and temporal variations of radon activity concentrations. Measurements require a large number of radon sensors with data loggers.

Our goal was to develop an inexpensive device with commercial photodiode for counting the alpha particles (in particular radon and its daughter elements). The principal operation of the developed monitoring system is based on the following steps: when a charged alpha particle hits the sensitive area of the sensor a small current is generated with amplitude proportional to the deposited energy. This current signal is converted into a voltage signal by a charge-sensitive preamplifier and amplified in several steps. Then the analogue signal is converted to digital by a comparator, and an ATmega328 microcontroller with a DS3231 RTC module is used to count and store the pulses. The alpha spectral response of the device has been calibrated by using 241Am solid source. Additionally, numerous tests were carried out in experimental chamber, with uranium ore sources. The developed detector was tested with several diffusion chambers with various sizes for soil gas and dwelling measurements, and determination of radon exhalation rate. Prototypes are currently being tested in deep boreholes, and in recultivated areas.

How to cite: Szabolcs, T., Ákos, H., and Kálmán, M.: Development of an active alpha particle detector for radon measurements, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13183, https://doi.org/10.5194/egusphere-egu25-13183, 2025.

      The second longest river in Europe along with its Delta (largest natural wetland) displays a sophisticated ecosystem with unique features which open the way for in-depth scientific research in the fields of geology, biology, ecology and many interdisciplinary subjects for which gamma-ray spectrometry is an essential technique. The Danube provides crucial data for raising awareness of the hazards induced by human activities, bringing significant contributions to improving methods and policies for environment preservation, wildlife protection and natural heritage conservation on a general basis, all of which being of great importance for science and society.

      Industrial pollution had a severe impact on air, water and soil/sediment quality. The TENORM nuclides dispersed in the atmosphere undergo dry/wet deposition, through complex sedimentation processes. Unsupported 210Pb and anthropogenic radioelements concentration data help identifying the periods during which radionuclides and pollutants acumulated in sediment strata. Long term averaged effects are comparable, but on shorter scales, any floods or comparable events induce perturbations. Consequently, any data complementary to physical and chemical determinations must be considered for this interdisciplinary approach to nuclear and environmental science, as the scope is performing retrospective investigations and further prediction making by studying gradient modifications in spatial and time coordinates.

            We perform low background adaptative and customized analysis with high efficiency&resolution detectors and dedicated software in order to face different environmental samples: our protocols have a general structure, but different approaches for different matrices, potential inhomogeneity, variable background, low/high count rates and related issues for detection limits and coincidence summing corrections. Experimental results and Monte Carlo simulations enable hypothesis testing for homogeneity and uncertainty issues. Additional neutron activation brings precious information from initially non emitting isotopes. Timing is crucial given the half-life of our main dating reference (210Pb): if the first sample sets from the course of the Danube are not measured quickly, the possibility of having time gradients for the beginning of the 20th century will be lost.

      The goal is developing a reference sediment data repository for mapping and analyzing radionuclide and pollutant dynamics, in order to be able to make predictions regarding the evolution of radionuclide concentration in addition to the retrospective analysis, for which we have dedicated methods and an associated software under patenting [1]. We bring a unitary methodology mainly governed by the IAEA recommendations, from sampling to measurements and calculations, including experimental protocols, intercomparison schemes and uncertainty budget optimization, in order to grow the sediment database we started and the associated interactive map [2], which displays priorly available data [3] and our first contributions [4-6]. The consortium under construction started with four labs from Romanian Universities and R&D Institutes. Enhancing this collaboration between Danube River Basin countries is our target at EGU25.

 

References

[1] Suvaila et al., Romanian Patent State Office A100734/2024

[2] www.blackforesea.eu

[3] available on request

[4] Suvaila et al., DOI 10.1007/s13762-024-06128-z

[5] Olacel et al., DOI 10.1016/j.chphi.2022.100065

[6] Pojar et al., Nuclear Technology & Radiation Protection 39 (3), 2024

How to cite: Suvaila, R.: Project Black: from Forest to Sea, Gamma-ray Analysis of Sediments from the Danube River, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20585, https://doi.org/10.5194/egusphere-egu25-20585, 2025.

EGU25-20863 | ECS | Orals | NH8.2

Radiological impact of the Tajogaite eruption (2021, La Palma, Canary Islands) 

Neus Miquel i Armengol, Alicia María Tejera Cruz, Ana del Carmen Arriola Velásquez, Claudio Briones Barrera, Héctor Eulogio Alonso Hernández, Jesús García Rubiano, and Pablo Martel Escobar

It is well known that volcanic eruptions represent an important source of natural radionuclide emissions into the environment; however, there are not many studies evaluating their radiological impact. The recent eruption of Tajogaite volcano, that took place in La Palma Island (Canary Islands, Spain) between September and December 2021, offers the opportunity to monitor its radiological impact on both the environment and the nearby population.
The eruption, located on the western site of Cumbre Vieja rift zone, lasted 85 days and large amounts of lavas and pyroclastic materials, along with fine lapilli and ash, were emitted. More than 1200 ha were covered by lava flows, destroying buildings and thousands of kilometres of roads, in addition to few hundred hectares of crop and farmland. The lava flows descended the western part of the island and finally reached the sea creating extensive lava deltas and platforms. As for the ashes, due to western winds, they also impacted the eastern side of the island. Moreover, emissions of radon gas were also detected. Although it is less known than other volcanic gases, its emission is significant due to its radioactive properties and potential health impact if it accumulates in enclosed spaces. In this work, the radioisotopic characterization of the products of the volcanic eruption is carried out, besides studying the possible radiological impact on the surrounding habitable areas. Activity concentrations of the main radionuclides of 238U, 235U and 232Th series, as well as 40K, have been determined from 40 samples of lava, xenopumices and ashes, by gamma and alpha spectrometry. These results have been analysed and compared with those previously obtained from the lavas of the underwater eruption on El Hierro Island in 2011, the Tagoro volcano. Furthermore, the radiological impact on the surrounding environment is also analysed from both measurements of terrestrial gamma radiation and the determination of the radioisotopic composition of soil samples. A total of 80 soil samples were collected and more than 150 measurements of terrestrial gamma radiation were taken during a campaign carried out in July 2023 around the entire island. Interpolation maps have been drawn using the ArcGIS Desktop 10.8.2 to represent the results obtained. The analysis of these maps identifies the areas near the eruption as areas of maximum activity concentration of 226Ra, as well as terrestrial gamma radiation. This trend significantly differs from results published in work prior to the eruption.

How to cite: Miquel i Armengol, N., Tejera Cruz, A. M., Arriola Velásquez, A. C., Briones Barrera, C., Alonso Hernández, H. E., García Rubiano, J., and Martel Escobar, P.: Radiological impact of the Tajogaite eruption (2021, La Palma, Canary Islands), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20863, https://doi.org/10.5194/egusphere-egu25-20863, 2025.

GI3 – Planetary Atmosphere and Ocean instrumentation system

EGU25-75 | ECS | Posters on site | PS1.3

Geomorphometric Assessment of the Marius Hill’s Pit for LunarLeaper 

Ramon Margarit, Anna Mittelholz, Valentin Bickel, and Simon Stähler

LunarLeaper is an ESA Small Mission candidate, aiming to robotically investigate lunar volcanic pits and associated subsurface lava tubes. Lunar pits likely represent collapsed ceilings of lava tubes, providing unique access to the lunar geologic record. One possible landing site for the LunarLeaper mission is the Marius Hills pit (MHP). The MHP is located within a sinuous rille in the region of Oceanus Procellarum (14.1ºN, 303.2ºE). Multiple exposed layers along the pit wall offer a unique opportunity to study the evolution of lunar volcanism, potentially revealing insights into the Moon's geological history. A thorough characterization of the lava tube may also pave the way for future human missions, as underground sites offer natural protection from the Moon's harsh surface conditions.

As part of the mission, the LunarLeaper, a legged robot, will explore the pit using high resolution cameras and possibly spectrometers, taking different images of the wall and the interior of the pit from different locations along the rim. Our main goals are to (1) characterize the slope and trafficability around the rim, (2) use the geomorphometry of the MHP to characterize and quantify viewing conditions, and (3) assess the need for and benefits of a mast-mounted camera. In this study, we use 3D point cloud reconstruction from Lunar Reconnaissance Orbiter Narrow Angle Camera images (Wagner and Robinson, 2022), to perform a geomorphometric assessment of the site. We analyze the slope and trafficability around the pit, which provides essential data in evaluating the robot’s ability to establish a line-of-sight with the pit wall and floor. Next, using ray-casting, we evaluate the overall visibility of the pit walls and floor if observed from the rim, exploring the balance between visibility/science return and the physical stability of the robot. Then, we identify optimal positions along the rim for which LunarLeaper can achieve a maximum level of visibility. In parallel, we evaluate the need for and benefits of a mast-mounted camera to enhance LunarLeaper’s ability to view into the MHP’s deep interior. Finally, we examine trade-offs between the slope angle traversed on the rim and mast height to achieve optimal visibility into the MHP while minimizing mission risk.

Our findings indicate that it is possible to capture depths down to 30 meters and on average 25 meters while remaining on low risk, i.e., less than 15 degree slopes. Additionally, using a relatively short mast (under 1 meter) enables the capture of the pit's deepest regions and the underlying lava tube. The outputs of this study will be used for mission design by providing input on (1) LunarLeaper design trade-offs, e.g., the possible addition of a camera mast, (2) the concept of operations e.g. with respect to path planning, and (3) the optimization of the scientific return of the overall mission.

How to cite: Margarit, R., Mittelholz, A., Bickel, V., and Stähler, S.: Geomorphometric Assessment of the Marius Hill’s Pit for LunarLeaper, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-75, https://doi.org/10.5194/egusphere-egu25-75, 2025.

EGU25-360 | ECS | Posters on site | PS1.3

Geologic and Thermophysical Characterization of Lunar Volcanic Pits 

Jordi Gómez Jodar, Anna Mittelholz, and Valentin Bickel

The LunarLeaper mission concept aims to explore subsurface lava tubes on the Moon. These are of interest for further robotic and human exploration, because such subsurface structures can provide shelter from the Moon’s hostile environment including radiation, large temperature fluctuations and micrometeorites. Satellite data has revealed that the lunar surface hosts hundreds of steep-walled pits. These pits have been hypothesized to represent collapsed ceilings of underground volcanic lava tubes, thus revealing unique insights into the subsurface and the geologic history of the Moon. Here, we characterize all currently known pit locations, as listed by Wagner and Robinson [2014], using globally available geologic, geomorphologic, and thermophysical information (from the Lunar Reconnaissance Orbiter LRO and the Selenological and Engineering Explorer SELENE). This enables us to map pit characteristics and relate them to the scientific, landing site, and operational requirements in the context of the LunarLeaper mission.

First, we study potential landing sites at each lunar pit considering that the rover will land in an area where the slope angle is smaller than 8° within a precision landing ellipse of 100 m. For each potential landing site, we quantify the visibility of the overall mission area, to determine if the robot would be able to establish line of sight with the lander antenna on the way to and once it reaches the volcanic pit. At the location with the best communication coverage, we evaluate the minimum distance to the pit, while considering slope and communication constraints. We also study the diurnal temperature variations which will set engineering requirements for the mission. Furthermore, we use the Unified Geological Map of the Moon, Fortezzo and Harrel [2020], to describe the geologic terrains hosting the pits. Finally, the characterization of all mapped lunar pits, allows us to perform an evaluation of landing sites most suited for LunarLeaper, while also providing constraints for any future missions targeting lunar pits.

 

References

Spudis P. D. Fortezzo, C.M. and S. L. Harrel. “Release of the digital Unified Global Geologic Map of the Moon at 1:5,000,000- scale.” In 51st Lunar and Planetary Science Conference, LPI Contribution, 2020. URL https://www.hou.usra.edu/meetings/lpsc2020/pdf/2760.pdf.

Robert V. Wagner and Mark S. Robinson. “Distribution, formation mechanisms, and significance of lunar pits.” Icarus, 237:52–60, 2014. ISSN 0019-1035. doi: https://doi.org/10.1016/j.icarus.2014.04.002. URL https://www.sciencedirect.com/science/article/pii/S0019103514001857.

How to cite: Gómez Jodar, J., Mittelholz, A., and Bickel, V.: Geologic and Thermophysical Characterization of Lunar Volcanic Pits, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-360, https://doi.org/10.5194/egusphere-egu25-360, 2025.

EGU25-566 | ECS | Orals | PS1.3

Constraining the distribution of radiogenics on the Moon from global geodynamic models 

Sabatino Santangelo, Ana-Catalina Plesa, Adrien Broquet, Doris Breuer, and Bart C. Root

The predominant concentration of volcanic activity and surface enrichment of heat producing elements (HPE) on the lunar nearside suggest an asymmetry in interior properties and thermal history of the Moon. The distribution of HPE beneath the surface and the processes that led to their enrichment on the nearside surface remain poorly understood (Gaffney et al., 2023). Interior radiogenic heating directly affects surface heat fluxes measured in situ during the Apollo program (Langseth et al., 1976), and estimated from orbit at the Compton-Belkovich (Siegler et al., 2023) and Region 5 locations (Paige & Siegler, 2016). 

Here, we link the subsurface distribution of HPE to the present-day surface heat flux using 3D thermal evolution models. We investigate the interior dynamics of the Moon from the post magma ocean crystallization phase to present-day using the mantle convection code GAIA (Hüttig et al., 2013). Similar to Plesa et al. (2016), we use a spatially variable crustal thickness model as input (Broquet & Andrews-Hanna, 2024). We investigate the structure of a putative HPE-rich layer underneath the PKT (Procellarum KREEP Terrane, Jolliff et al., 2000) assuming a circular geometry. We vary its location, size, depth and HPE enrichment compared to the mantle and anorthositic crust. Our models consider the HPE concentrations as constrained from magma ocean crystallization studies, but assume that additional mechanisms may have led to a migration of heat sources below the PKT region. 

Similar to Laneuville et al. (2013), we find that an enriched layer placed below the crust can efficiently heat up the mantle and contribute to explaining prolonged lunar magmatism. We show that the prominent gravity anomaly associated with the warm mantle beneath the PKT (Laneuville et al., 2013; Grimm, 2013) can be used to construct updated crustal thickness models, which display a substantially thinner nearside crust.

Our models show that a large HPE anomaly underneath PKT (~1500 km radius) allows sufficient surface heat flux variability to account for the low Region 5 value (Paige & Siegler, 2016) and the Apollo 15 & 17 measurements (Langseth et al., 1976). Conversely, a smaller anomaly (<1200 km) fails to produce any significant difference in surface heat flux between Apollo 17 measurement and Region 5 estimate. However, this geometry may help explain the absence of Imbrium’s western ring (Broquet & Andrews-Hanna, 2024) and the spatial variability in the relaxation state of lunar basins (Ding & Zhu, 2022).

Our models provide an important baseline for the interpretation of upcoming heat flux measurements within Mare Crisium (TO19D, Nagihara et al., 2023) and Schrödinger Crater (CP-12, Nagihara et al., 2023), predicting that the heat flux at Crisium and Schrödinger should be comparable to that measured at Apollo 17 and estimated at Region 5, respectively. Significantly different heat flux measurements would have profound implications for our understanding of the distribution of radiogenic elements within the lunar interior. Lastly, quantifying the subsurface thermal state and the distribution of HPE on the Moon will prove crucial for infrastructure development in the framework of the Artemis program. 

How to cite: Santangelo, S., Plesa, A.-C., Broquet, A., Breuer, D., and Root, B. C.: Constraining the distribution of radiogenics on the Moon from global geodynamic models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-566, https://doi.org/10.5194/egusphere-egu25-566, 2025.

EGU25-691 | Orals | PS1.3

High-resolution surface temperatures of the Moon derived from Imaging Infra-Red Spectrometer (IIRS) on-board Chandrayaan-2: A case study on the Schrödinger Basin 

Subhadyouti Bose, Denesh Karunakaran, Tvisha Kapadia, Neha Panwar, and Neeraj Srivastava

Imaging Infra-Red Spectrometer (IIRS), sent on-board Chandrayaan-2, has been mapping the lunar surface since 2019 with high spatial (80 m/pixel) as well as spectral resolutions (0.7 to 5 µm) [1-3]. This study uses two IIRS images, portions of which encompass the floor of Schrödinger Basin. Surface temperatures were derived from the two overlapping IIRS strips, which were then used to study the thermal properties of a part of the basin’s floor. Additionally, surface temperatures were also acquired by processing corresponding Diviner data, by matching IIRS pixels according to their Ground Control Points (GCPs) along with their local times of acquisition. It has been deduced that, for a particular period of time, the temperatures derived from IIRS are comparable with the corresponding Diviner data. Furthermore, factors contributing towards the mean temperature differences between the IIRS and Diviner datasets have been identified.

In order to use the temperatures obtained from IIRS, a case study on the ~320-km-wide-Schrödinger Basin was performed. In this regard, a volcanic vent (Schrödinger G), situated at 75° S and 139° E was studied, which is known to have deposited pyroclastic material on the basin floor [4-5]. Our analysis on the pyroclastic material-covered surface around the vent reveals several interesting findings: (1) Using the temperature data from IIRS, we were able to identify two distinct morphological units within the same pyroclastic deposit. The two units surrounding the vent exhibit different surface temperatures (an average relative difference of ~25-30K). (2) We have also used Clementine UVVIS colour-ratio data to identify differences related to soil mineralogy across the two deposits. The two units display contrasting tonal signatures on the UVVIS FCC image, thereby confirming the presence of two mineralogically distinct surface units. (3) In addition, using images from LRO-NAC, we have also performed a crater size frequency distribution (CSFD) measurement on the two units to estimate their relative ages. Our analysis reveals that the vent has experienced multiple eruptions, with the oldest ~3.7 Ga ago, while the latest being ~1.8 Ga ago, interspersed with different eruptions in between. Furthermore, CSFD measurements reveal that one of the units is significantly younger than the other. Based on the above results, we attribute the deposition of materials with different textures on either side of the vent to the several episodes of eruptions.

In conclusion, due to IIRS’s relatively higher spatial resolution, it was possible to identify and establish significant differences within a single pyroclastic deposit on the basis of derived temperature data, which have been validated from spectroscopic data as well. This study thus highlights the importance of using high-resolution IIRS data for such studies in future.

References: [1] Chowdhury et al. 2020, Current Science, 118, 368–375. [2] Bose et al. 2024, Advances in Space Research, 73, 2720-2752. [3] Verma et al. 2022, Icarus, 383, 115075. [4] Kramer et al. 2013, Icarus, 223, 131-148. [5] Kring et al. 2021, Advances in Space Research, 2021, 4691-4701.

How to cite: Bose, S., Karunakaran, D., Kapadia, T., Panwar, N., and Srivastava, N.: High-resolution surface temperatures of the Moon derived from Imaging Infra-Red Spectrometer (IIRS) on-board Chandrayaan-2: A case study on the Schrödinger Basin, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-691, https://doi.org/10.5194/egusphere-egu25-691, 2025.

EGU25-1505 | Posters on site | PS1.3

JAXA Virtual Planet: A next-generation web-GIS platform for lunar data visualization and analysis 

Ryodo Hemmi, Hiroyuki Sato, Shoko Oshigami, Shingo Nanbu, and Mitsuo Yamamoto

JAXA Virtual Planet (VP) system, developed by JAXA Lunar and Planetary Exploration Data Analysis Group (JLPEDA), is an innovative Web-GIS platform based on ESRI’s ArcGIS suite. Started in 2020, VP serves as the successor to Kaguya Integrated Data Analysis System (KADIAS), enhancing visualization and analysis capabilities of lunar data. Unlike KADIAS, which was limited to 2D visualizations, VP supports global 3D spherical visualization with topography, as well as 2D and 3D views of polar and mid-latitude regions. One of VP’s standout features is a bird’s-eye view functionality, which enables dynamic perspective changes in 3D visualizations.

VP is available in two versions: Easy version, designed for general users with an emphasis on accessibility and mobile compatibility, and Advanced version, which caters to researchers with advanced analytical tools. VP integrates both publicly available Kaguya mission datasets (e.g., PDS data products) and proprietary high-level processed datasets, such as FeO/TiO2 content maps and lunar mare age maps, offering a comprehensive platform for lunar exploration data analysis.

Key features of VP include:
1.    Distance and area measurement,
2.    Shareable URLs for reproducing screen states,
3.    Pop-up attribute information for layers,
4.    Custom visualizations (e.g., RGB composition, arithmetic operations, and color mapping),
5.    Cross-section visualization and download (3D view only),
6.    Location nomenclature search,
7.    Sun and Earth sub-point display,
8.    Drawing and memo input,
9.    Printing, and
10.    Data downloads for user-defined regions.

Features (4) through (10) are exclusive to the Advanced version, designed to meet the needs of researchers. Compared to KADIAS, VP introduces several new functions, significantly enhances usability, and improves data resolution. These advancements mark a substantial leap forward in functionality and user experience, allowing for more detailed and flexible analyses of lunar datasets.

VP is currently undergoing final revisions (e.g., accelerating Kaguya Spectral Profiler data rendering, generating cache data for ArcGIS map image layers, addressing bug fixes, etc.) for public release, which is scheduled to occur within the current fiscal year. This system aims to become an essential tool for lunar and planetary science community, offering enhanced capabilities for both general users and researchers.

How to cite: Hemmi, R., Sato, H., Oshigami, S., Nanbu, S., and Yamamoto, M.: JAXA Virtual Planet: A next-generation web-GIS platform for lunar data visualization and analysis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1505, https://doi.org/10.5194/egusphere-egu25-1505, 2025.

EGU25-2927 | Orals | PS1.3

Potential Survivable Niches for Microbial Life on the Lunar South Pole 

Prabal Saxena, Stefano Bertone, Heather Graham, Natalie Curran, Aaron Regberg, Andrew Needham, Betsy Pugel, and Noah Petro

The surface conditions on most of the lunar surface are incredibly harsh for survival of microbial life. Combinations of high doses of ultraviolet radiation, high temperatures, and energetic particle radiation are likely to limit survival over most unprotected surfaces on the Moon. This is particularly true in equatorial regions, where all previous crewed exploration of the Moon has taken place. However, whether these surface conditions are as widespread at high latitude regions such as the lunar poles has not been examined while considering the effect of topography.  Comparing topography and latitude-driven surface conditions using remote sensing data and high-resolution models of illumination conditions in lunar polar regions to survivability data of specific microorganisms, we find that there are significant areas in the lunar poles that likely possess surface conditions amenable to the survival of those microbes. The potential survivability of microbial life at the lunar poles is particularly significant given the numerous plans for crewed exploration of the lunar south pole in the near future. Additionally, many of the microbes we examined are likely to be brought to the Moon as a side effect of crewed exploration. Thoughtfully planning exploration and tracking its impact in this context is key to limiting and understanding potential unintended transfer of life to the Moon.

How to cite: Saxena, P., Bertone, S., Graham, H., Curran, N., Regberg, A., Needham, A., Pugel, B., and Petro, N.: Potential Survivable Niches for Microbial Life on the Lunar South Pole, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2927, https://doi.org/10.5194/egusphere-egu25-2927, 2025.

EGU25-3659 | Posters on site | PS1.3

LunarLeaper - Unlocking a Subsurface World 

Simon C. Stähler, Anna Mittelholz, Hendrik Kolvenbach, Philip Arm, Valentin Bickel, Joseph Church, Svein-Erik Hamran, Adrian Fuhrer, Michael Gschweitl, Elena Krasnova, Ramon Margarit, Jordan Aaron, Sofia Coloma, Matthias Grott, Marco Hutter, Ozgur Karatekin, Miguel OIivares-Mendez, Birgit Ritter, Johan Robertsson, and Krzysztof Walas

LunarLeaper is a mission concept designed to robotically explore subsurface lava tubes on the Moon. Lunar pits, steep-walled collapse features, are thought to be connected to such lava tube systems and more than 300 have been identified through remote sensing. These natural subsurface structures hold immense value for exploration and scientific investigations, because they offer protection from radiation, micrometeorites, and harsh temperature fluctuations on the lunr surfac

e and as such, they have been proposed for possible future human habitation. In addition, the extent, nature and duration of lunar volcanism is poorly understood and the uniquely exposed stratigraphy along the pit walls might hold crucial
information on the volcanic history if the Moon.

However, current orbital imaging lacks sufficient resolution to confirm these connections, making ground-truth exploration essential. LunarLeaper aims to address these knowledge gaps by deploying a lightweight (<15 kg) legged robot capable of autonomously traversing challenging terrains, including steep slopes and boulder fields, that hinder traditional wheeled rovers. The mission will investigate four primary objectives:

  • (1) Subsurface Lava Tubes—confirming the presence and extent of lava tubes;
  • (2) Suitability for Human Habitation—assessing the accessibility stability of pits;
  • (3) Geological Processes—analyzing the exposed stratigraphy along pit walls to study volcanic evolution, the number and timing of lava flows, and the compositional evolution of the lunar interior;
  • (4) Regolith Assessment—exploring the lateral and vertical extent of regolith, which holds vital information about the Moon’s geological and impact history.

The legged robot will land close to a lunar pit, equipped with ground-penetrating radar (GPR) and a gravimeter to map subsurface structures and detect lava tubes. It will also capture high-resolution images and compositional data from the pit walls travelling a total of approximately 1 km within one lunar day (approximately 12 Earth days). LunarLeaper not only advances lunar exploration by providing access to previously unreachable terrains but
also demonstrates the potential of legged robotic systems in space. It will serve as a key technology demonstration, contributing to the development of future robotic exploration systems and laying the groundwork for future human missions to the Moon.

How to cite: Stähler, S. C., Mittelholz, A., Kolvenbach, H., Arm, P., Bickel, V., Church, J., Hamran, S.-E., Fuhrer, A., Gschweitl, M., Krasnova, E., Margarit, R., Aaron, J., Coloma, S., Grott, M., Hutter, M., Karatekin, O., OIivares-Mendez, M., Ritter, B., Robertsson, J., and Walas, K.: LunarLeaper - Unlocking a Subsurface World, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3659, https://doi.org/10.5194/egusphere-egu25-3659, 2025.

EGU25-4290 | ECS | Orals | PS1.3

Effects of the South Pole-Aitken Magnetic Anomaly Cluster on the Plasma Environment at the Lunar South Pole 

Thomas Maynadié, Yoshifumi Futaana, Stas Barabash, Anil Bhardwaj, Peter Wurz, and Kazushi Asamura

Despite lacking a global magnetic field, the Moon features localized magnetized regions called lunar magnetic anomalies [1]. Their interaction with the solar wind results in significant proton reflection and deflection [2], creating unique structures often referred to as lunar mini-magnetospheres [3, 4]. Previous studies have shown that the largest magnetic anomaly, the South Pole-Aitken (SPA) cluster, induces global-scale perturbations in the near-surface lunar plasma environment on both the dayside [5, 6] and nightside [7]. However, its influence on the plasma environment in south polar regions remains unknown.

In this study, we produce new composite images of backscattered energetic neutral hydrogen derived from Sub-KeV Atom Reflecting Analyzer (SARA) [8] data. These images reveal that plasma perturbations generated by the SPA cluster can extend to lunar south-polar regions, depending on local time and upstream solar wind conditions. These perturbations affect solar wind proton precipitation patterns, either decreasing or enhancing impinging proton fluxes depending on whether the south pole lies downstream or outside of the SPA anomaly. Based on these observations, we develop an empirical model of solar wind compression by the SPA cluster to evaluate its impact on ion instrument measurements at the south pole.

Understanding the complex interactions between the plasma, dust, and electromagnetic environments is an important asset to ensure safe and sustainable human presence on the Moon. We will discuss the role of the SPA cluster in these interactions, which will establish preliminary measurement requirements for in-situ plasma instruments in polar regions.

References:

[1] Coleman et al. (1972), Physics of the Earth and Planetary Interiors, https://doi.org/10.1016/0031-9201(72)90050-7.

[2] Lue et al. (2011), Geophysical Research Letters, https://doi.org/10.1029/2010GL046215.

[3] Lin et al. (1998), Science, https://doi.org/10.1126/science.281.5382.1480.

[4] Wieser et al. (2010), Geophysical Research Letters, https://doi.org/10.1029/2009GL041721.

[5] Fatemi et al. (2014), Journal of Geophysical Research: Space Physics, https://doi.org/10.1002/2014JA019900.

[6] Maynadié et al. (2024), Europlanet Science Congress 2024, Berlin, https://doi.org/10.5194/epsc2024-79.

[7] Dhanya et al. (2018), Geophysical Research Letters, https://doi.org/10.1029/2018GL079330.

[8] Barabash et al. (2009), Current Science, http://www.jstor.org/stable/24105464.

How to cite: Maynadié, T., Futaana, Y., Barabash, S., Bhardwaj, A., Wurz, P., and Asamura, K.: Effects of the South Pole-Aitken Magnetic Anomaly Cluster on the Plasma Environment at the Lunar South Pole, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4290, https://doi.org/10.5194/egusphere-egu25-4290, 2025.

EGU25-4338 | Orals | PS1.3

Nano-geochemical insights into the source of lunar metals 

Phillip Gopon, James Douglas, Michael Moody, Alexander Halliday, Bernard Wood, and Jon Wade

Although metallic iron (Fe0) is a ubiquitous product of space weathering, its formation mechanisms are still poorly understood. On the lunar surface, Fe0 particles ranges in size from a few nm to several mm and are widely believed to have formed by a variety of mechanisms. These include the in-situ reduction of FeO during cosmic ray bombardment, localized heating by micrometeorites and the subsequent reduction of FeO, as well as the addition of Fe0 from iron-nickel meteorites during micrometeorite bombardment (Hapke, 2001; Kuhlman et al., 2015; Gopon et al., 2017; Day, 2020). The exact formation mechanism has wide ranging implications for remote spectral analysis of airless planetary bodies, the cosmic ray and micrometeorite flux to the Moon, correction of bulk-geochemical data on the moon, and the potential of the lunar surface to be a source of critical metals.

We present the results of a combined Electron Probe Micro-Analyses (EPMA) and Atom Probe Tomographic (APT) study to characterize the composition of Fe0 from Apollo 16 Regolith (sample #61500). Combining these techniques allowed us to explore the wide range of textural occurrences and size fractions of Fe0 and constrain the origin and emplacement mechanisms of these metallic regolith components. We focused on the germanium, iron, and nickel concentrations of the Fe0, as these three elements are key tracers that enable differentiation of in-situ vs extra-lunar processes. Our work shows that all Fe0 analysed in sample 61500 exhibit a meteoritic geochemical signature, which is most closely linked to the IIAB group of iron meteorites  (Gopon et al., 2024). This rare meteorite group is notable for its low nickel but high germanium concentrations. The lunar regolith’s significant inventory of meteoritic metals implies that it is a potentially valuable resource for a range of critical metals (EU Report, 2023), not least the Pt group metals and germanium. Furthermore, the host phase – npFe –contained within powdered regolith implies extraction and refining of these elements might be significantly more energy and cost effective than terrestrial deposits.

 

References:

Day, J.M.D., 2020, Metal grains in lunar rocks as indicators of igneous and impact processes: Meteoritics and Planetary Science, v. 15, doi:10.1111/maps.13544.

EU Report, 2023, Study on the Critical Raw Materials for the EU 2023 – Final Report:

Gopon, P., Douglas, J.O., Gardner, H., Moody, M.P., Wood, B., Halliday, A.N., and Wade, J., 2024, Metal impact and vaporization on the Moon’s surface: Nano-geochemical insights into the source of lunar metals: Meteoritics & Planetary Science, v. 59, p. 1775–1789, doi:10.1111/maps.14184.

Gopon, P., Spicuzza, M.J., Kelly, T.F., Reinhard, D., Prosa, T.J., and Fournelle, J., 2017, Ultra-reduced phases in Apollo 16 regolith: Combined field emission electron probe microanalysis and atom probe tomography of submicron Fe-Si grains in Apollo 16 sample 61500: Meteoritics & Planetary Science, v. 22, p. 1–22, doi:10.1111/maps.12899.

Hapke, B., 2001, Space Weathering from Mercury to the asteroid belt: Journal of Geophysical Research, v. 106, p. 39–73.

Kuhlman, K.R., Sridharan, K., and Kvit, A., 2015, Simulation of solar wind space weathering in orthopyroxene: Planetary and Space Science, p. 1–5, doi:10.1016/j.pss.2015.04.003.

How to cite: Gopon, P., Douglas, J., Moody, M., Halliday, A., Wood, B., and Wade, J.: Nano-geochemical insights into the source of lunar metals, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4338, https://doi.org/10.5194/egusphere-egu25-4338, 2025.

EGU25-6383 | Posters on site | PS1.3

Proclus crater: a study case to integrate compositional information and morpho-stratigraphic mapping on the Moon 

Cristian Carli, Lorenza Giacomini, Giovanna Serventi, and Maria Sgavetti

Geological planetary mapping is mainly done by considering morphology and stratigraphic information, supported sometimes by color variation to define boundaries of superficial textures or highlight physical properties. In recent years more attention was used to integrate mineralogical indications from the visible to the near-infrared (VNIR) to the usual planetary geological mapping. Specifical examples has been tested on Mercury (e.g. Wrigth et al., ESS, 2024), on Mars (e.g. Giacomini et al., Icarus, 2012) and on the Moon (e.g. Tognon et al., JGR, 2024).

Here, we investigate the Proclus crater, a 28 km, simple and fresh crater, Copernican in age (Apollo 15 PSR), which shows a variegate VNIR reflectance properties. We have analyzed the M3 m3g20090202t024131 (onboard Chandrayaan-1 mission) image to study the composition of Proclus crater whereas a mosaic compiled with six LROC (Lunar Reconnaissance Orbiter Camera) NAC images, with a spatial resolution of 0.8 m/pixel, has been used to define the morpho-stratigraphic map of the area.

We first classified the crater in different spectral regions applying the Spectral Angle Mapper (Kruse et al., REMOTE SENS. ENVIRON., 1993) method and using image-driven end-members by Purity Pixel Index (PPI, Boardman,  7JPL-Air.Geos.W., 1993). PPI supports the definition of 7 end-members, integrated by other 4 end-members evaluating the spectral variability.

Representative spectrum of each Spectral Unit was deconvolved by Gaussian model and results on mineralogical detection were compared with well characterized terrestrial analogues. The 11 end-members support the definition of six main Spectral Units and 2 units were divided in sub-units from a mineralogical point of view.  The Spectral Units recognized from Proclus crater indicate that this crater is characterized by lithologies rich in plagioclase mixed with variable amount of different mafic phases.

Geomorphological mapping highlights as Proclus crater walls is affected by mass wasting deposits, mainly represented by taluses. The crater floor is instead dominated by impact melt with different surface texture: from smooth melt ponds to more hummocky and knobby deposits.

Finally, Spectral Units were used to improve the morpho-stratigraphic map and identify sub-units or new-units.

We acknowledge support from the Horizon 2020 program grant agreements 871149-GMAP and 776276-PLANMAP.

How to cite: Carli, C., Giacomini, L., Serventi, G., and Sgavetti, M.: Proclus crater: a study case to integrate compositional information and morpho-stratigraphic mapping on the Moon, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6383, https://doi.org/10.5194/egusphere-egu25-6383, 2025.

EGU25-6664 | ECS | Orals | PS1.3

Volatile Ice Presence Analysis through Mass Wasting Events Mapping in Lunar Permanently Shadowed Regions 

Riccardo Pedrelli, Valentin Bickel, Jordan Aaron, and Ariel Deutsch

Mass wasting events on the Moon have been documented since the Apollo era and are distributed across its surface. On Earth, the morphology and runout distance of landslides, particularly flowlike landslides such as debris and mud flows, are strongly influenced by the mobilized soil and bedrock properties, notably the water content.

Despite the absence of widespread, liquid surface water on the Moon, previous surveys identified numerous lunar flow events across the Moon’s equatorial regions (± 60° latitude), termed “granular flows” or “flows”, in short, excluding the polar regions due to unfavorable illumination conditions. The recent release of ShadowCam images now enables the extension of past mapping efforts to the shadowed portions of the lunar polar regions (> 80° latitude).

Here, we perform a thorough, manual search for flows in polar region craters using images from the Korean Pathfinder Lunar Obiter (KPLO) ShadowCam and the Lunar Reconnaissance Orbiter (LRO) Narrow Angle Camera (NAC). We analyzed three regions for comparison: the Equatorial Region (Eq) (±60°), the South Pole Region (Sp) (80°–90° S), and the North Polar Region (Np) (80°–90° N). We focused our mapping efforts on flows in craters where more than 1% of the internal area has slope angles exceeding 30°. We utilized 131 ShadowCam images and 84 processed NAC images to map flows. Additionally, 100 random highland events from the Eq region were manually mapped for comparison with polar events.

We identified 23 Sp and 99 Np flows, distributed across 3 and 16 craters, respectively. A significant disparity emerged between the Eq and polar regions. While 38.7% of craters with slopes exceeding 30° in the Eq region contained flows, the percentages dropped to 33.3% in Np and 16.6% in Sp. Consequently, the likelihood of developing flows in Np and Sp with the same distribution as the Eq region is only 8.02% and 0.59%, respectively. Notably, Sp flows occur in areas with relatively lower LPNS-derived Water Equivalent Hydrogen (WEH) and outside permanently shadowed regions (PSRs) compared to Np flows. We observe no significant differences in geomorphic flow characteristics between the three regions. Flow efficiency (flow height/length, or H/L) averaged ~0.6, and the median source angle was ~32° across all regions.

Our results suggest that flows are 1) scarce in the polar regions, yet 2) do not exhibit anomalous geomorphologic properties in comparison to equatorial (dry) flows. This suggests the presence of an inhibitory factor - or the absence of the pre-conditions required for flow formation. Ongoing work is investigating whether our observations could be explained by a cementing effect caused by (near-)surface volatiles. The accumulation of volatiles might strengthen the regolith, reducing the probability of flow initiation due to meteorite-induced seismicity or moonquakes. Our observations might also indicate that potentially large quantities of subsurface volatiles are not shallow enough to cause and/or become mobilized in flow events. It is also possible that the observed flows formed before volatiles accumulated.

How to cite: Pedrelli, R., Bickel, V., Aaron, J., and Deutsch, A.: Volatile Ice Presence Analysis through Mass Wasting Events Mapping in Lunar Permanently Shadowed Regions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6664, https://doi.org/10.5194/egusphere-egu25-6664, 2025.

High-speed impacts are the most fundamental of the currently known geological process in the Solar System. Luna preserves a comprehensive record of impacts since its formation 4.53 billion years age (Ga). Particles of silicate glass formed by impact melting may have recorded the timing of the impact event and reflected the composition of crustal target materials. Previous studies have used 39Ar-40Ar and U-Pb chronometric systems to date lunar impact glasses, while their source characteristics were assessed using major and trace element data. The return of the Chang'e 5 sample provides an opportunity for a more comprehensive analysis of lunar impact history by comparing the ages of impact glasses from different locations.

 

In this study, we collected approximately 800 sets of isotopic age data and corresponding major and trace element data for impact glasses, primarily from samples returned from the Apollo series of missions and the recent Chang’e 5 mission. Impact glasses for which no age data could be obtained were removed. Impact flux curves were generated by normalizing the estimated age data. Sampling points on the lunar nearside show three distinct curve patterns. The impact flux curves of Chang'e 5 and Apollo 12 exhibit a common, prominent impact interval during the lunar Copernicus Period. The impact flux curves based on the Apollo 17 samples show only one prominent impact interval, namely the Late Heavy Bombardment (LHB) Event period (3.8-4.1 Ga). The intermediate region samples (Apollo 14, 15,16) exhibit both of these common, prominent impact intervals. These three impact flux curve patterns may be related to the geographic distribution of the sampling sites. To validate this potential relationship, we utilized a global catalog of lunar impact craters containing over 1.3 million craters to analyze the distribution of craters of similar diameter in contemporary regions. Preliminary results indicate that there are differences in the distribution of impact craters across different regions within the same geological period. These differences may be related to the Moon's rotation and orbital characteristics. 

How to cite: zhao, S. and fan, J.: Geospatial analysis of lunar impacts craters: a meta-analysis of impact glasses from all Apollo and Chang'e 5 missions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7589, https://doi.org/10.5194/egusphere-egu25-7589, 2025.

EGU25-8214 | Posters on site | PS1.3

Lunar In-situ Navigation and Communication Node - LUNINA 

Antti Kestilä, Harri Haukka, Ignacio Arruego, Ari-Matti Harri, Maria Genzer, Victor Apéstigue, Maria Hieta, Carmen Camañes, Cristina Ortega, Jarmo Kivekäs, and Petri Koskimaa

LUNINA is an in-situ navigation and communication node. The proposed platform is designed to be a compact, independent, cost effective, robust, and location independent navigation beacon and communication relay on the Moon that can operate 24/7. The design draws from the European Space Agency (ESA)-funded MiniPINS LINS platform [1], developed for long-term deployment in the Schrödinger crater but adaptable to other lunar environments with sufficient sunlight. Each LINS unit incorporates a Radioactive Heating Unit (RHU) to maintain functionality during the cold lunar night and uses solar panels and batteries for continuous power.

LUNINA serves two primary purposes: navigation and communication. As a navigation aid, each node emits signals that support line-of-sight users on the  surface and orbiting spacecraft, providing critical assistance for tasks such as landing and launch operations. When deployed at elevated locations, the nodes enhance surface navigation by offering precise positioning. For communication, LUNINA functions as a relay for data transfer between ground and orbit-based users. The elevated placement of nodes allows them to cover larger surface areas and relay messages through a network configuration. This capability supports both localized communication near lunar bases and broader applications across the Moon's surface.

Figure 1: LUNINA nodes (in red dots) in Schrödinger crater around the Lunar Base (green dot).

The platform functions as a durable communication and navigation network for lunar missions. The default payload for LUNINA is a communication system, which facilitates seamless integration into lunar infrastructure. Designed as a "drop and forget" solution, the system offers long-term reliability for safe and flexible lunar exploration.

Figure 2: Different applications of the LUNINA node.

The inclusion of an RHU would allow the thermalization of the in-situ LUNINA unit during the Lunar night, where energy storage need may lead to unaffordable battery volumes. Radioisotope power systems utilising americium-241 as a heat source fuel have been under development in Europe since 2009 as part of a European Space Agency funded programme [2].

The LUNINA platform will support multiple navigation methods, including ranging and range-rate measurements. Utilizing signals from multiple nodes enhances navigational accuracy for landing and launch operations. As part of the broader Lunar Communications and Navigation Services (LCNS) initiative, the system’s modular design allows for future upgrades to maintain compatibility with evolving infrastructure.

Key Features:
1. Compactness: Derived from the MiniPINS LINS platform.
2. Independence: Capable of continuous 24/7 operation.
3. Cost-Effectiveness: Using the heritage LINS, standardized parts and systems, the costs of development is minimized. Once node is developed, the node can be mass produced, bringing down its cost.
4. Robustness and Modularity: Supports standardized interfaces and updatable software.
5. Durability: Designed for long-term operation with upgradable software.
6. Location Independence: Deployable anywhere on the Moon.


References:
[1] Genzer M., et al. "MiniPINS - Miniature Planetary In-situ Sensors," EGU General Assembly 2021, https://doi.org/10.5194/egusphere-egu21-11282.

[2] Ambrosi et al., "European Radioisotope Thermoelectric Generators (RTGs) and Radioisotope Heater Units (RHUs) for Space Science and Exploration," Space Sci Rev 215, 55 (2019), https://doi.org/10.1007/s11214-019-0623-9.

 

How to cite: Kestilä, A., Haukka, H., Arruego, I., Harri, A.-M., Genzer, M., Apéstigue, V., Hieta, M., Camañes, C., Ortega, C., Kivekäs, J., and Koskimaa, P.: Lunar In-situ Navigation and Communication Node - LUNINA, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8214, https://doi.org/10.5194/egusphere-egu25-8214, 2025.

EGU25-8239 | Orals | PS1.3 | Highlight

SER3NE - A small orbiter mission to the Moon 

Stephanie C. Werner and the The SER3NE Team

Selene’s Explorer for Roughness, Regolith, Resources, Neutrons and Elements (SER3NE) is a small satellite mission performing gamma-ray and neutron spectroscopy (University of Oslo), near-infrared spectroscopy (Royal Observatory of Belgium and Royal Belgian Institute for Space Aeronomy) , and laser altimetry, roughness, and albedo observations (Institute for Planetary Reserch - DLR) at unprecedented spectral and ground resolution. The aim is to characterize the lunar surface to unravel its volatile origin and delivery processes, to uncover the geological processes that shaped the Moon, to prospect lunar resources for ISRU at future landing sites, to determine the exact neutron lifetime and the orbital evolution of the Earth-Moon system.
The instruments will be carried by the modular, single-failure tolerant TUBiX20 satellite platform (Technical University of Berlin). To ensure the desired global coverage and resolution for all instruments the satellite will orbit the Moon on a eccentric polar orbit with a slowly, naturally drifting argument of perilune over the mission lifetime of one year. This mission concept is a pre-Phase A Study led by University of Oslo under an ESA contract.

How to cite: Werner, S. C. and the The SER3NE Team: SER3NE - A small orbiter mission to the Moon, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8239, https://doi.org/10.5194/egusphere-egu25-8239, 2025.

    Planetary seismic data are essential for studying planetary interiors and dynamics, yet acquiring high-quality recordings in harsh extraterrestrial environments turns out to be far more challenging than on Earth. In both the Apollo Passive Seismic Experiment on the Moon and the Seismic Experiment for Interior Structure (SEIS) on Mars, considerable transient disturbances—often referred to as “glitches”—span a wide range of frequencies, complicating the search for potential low-frequency signals of planetary free oscillations and gravitational wave responses. To address this issue, we propose an automated workflow for detecting and removing strong transient disturbances in Apollo seismic data with deep learning, thereby enhancing the recovery of weak long-period signals. We also examined two approaches for removing disturbance: (1) directly muting transient segments and applying Fourier transforms, and (2) treating these segments as data gaps and applying the Lomb–Scargle periodogram to uncover weak low-frequency signals. Synthetic tests show that even with ~80% of the data contaminated, most low-frequency peaks can still be recovered. Moreover, our workflow recovers the recently discovered temperature-related long-period signals in Apollo data without relying on stacking or clustering techniques, highlighting its vast potential in revisiting low-frequency components of Apollo seismic data.

    Complementing this disturbance-mitigation framework, we also evaluate the phasor walkout method, which determines whether a spectral peak originates from a true signal or merely from noise. The core assumption of this method is that harmonic signals will generate linear walkout patterns at their true frequency peaks, while random noise will produce irregular, random walkout paths. However, our findings indicate that random noise can contain a considerable amount of frequency peaks with deceptively linear phasor walkout patterns. Although noise in planetary seismic data are not random Gaussian noise, and artifacts observed in simple random noise may or may not arise in actual lunar or Martian data, this finding nonetheless highlights the need for extra caution when interpreting phasor walkout results in planetary seismic data.

    In summary, our study offers both an effective strategy for strong-disturbance removal—enabling the search for weak low-frequency signals—and an assessment of the phasor walkout method, raising awareness of risks in potential misinterpretations. These insights not only open new avenues for re-examining legacy Apollo data but also provide gentle reference in detecting planetary free oscillations and other low-frequency seismic signals.

How to cite: Xiao, Z. and Li, J.: Apollo Lunar Seismic Data Disturbance Mitigation and Phasor Walkout Method Assessment for Searching Planetary Free Oscillations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8502, https://doi.org/10.5194/egusphere-egu25-8502, 2025.

Apollo lunar seismic data are essential for understanding the Moon’s internal structure and geological history. Despite being collected over five decades ago, the Apollo dataset remains the only available source of lunar seismic data, continuing to provide valuable insights into the interior of the Moon and its seismic activity. Recent advances in artificial intelligence, particularly deep learning techniques, have significantly enhanced planetary seismology by providing novel and powerful methods for analyzing previously under-explored, or even unrecognized seismic signal types. In this study, we apply deep learning for unsupervised clustering of lunar seismograms, revealing a new kind of long-period seismic signal that persisted every lunar night from 1969 to 1976. Through a detailed analysis of its timing, frequency, polarization, and temporal distribution, we concluded that this signal is likely induced by the cyclic heater, rather than being an artifact of voltage changes or other artificial sources. In addition to this newly identified signal, the unsupervised clustering algorithm also revealed a class of step/spike signals in acceleration (ACC-Step/Spike) similar to calibration signals. We built a comprehensive search of these signals using template matching, and then analyzed their features. These signals are particularly prevalent during lunar sunrise, sunset, and noon, and their amplitude range varies with temperature as well. Unlike the calibration signals with linear polarization, these ACC-Step/Spike signals exhibit elliptical polarization. Their incidence angles occasionally show noticeable variation during sunrise and sunset. Their characteristics in terms of azimuth and incidence angles also exhibit significant differences between the vertical and horizontal components. For example, in the horizontal component, the azimuth distribution is relatively uniform, and the incidence angle is nearly vertical. In contrast, in the vertical component, the azimuth distribution is sometimes more stable, and the incidence angle distribution is more uniform. Furthermore, our clustering results uncovered short-period abnormal signals near lunar noon and those caused by instrument malfunctions. Our research introduces a novel method for discovering new types of planetary seismic signals and enhances our understanding of Apollo seismic data. The discovery of long-period signals and the ACC-Step/Spike catalogs provide valuable references for future lunar seismic observations and data interpretation, thereby benefiting the analysis of lunar seismic signals.

How to cite: Liu, X. and Li, J.: Searching for Under-Explored Signals in Apollo Seismic Data by Deep Learning and Template Matching, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9482, https://doi.org/10.5194/egusphere-egu25-9482, 2025.

EGU25-11607 | Orals | PS1.3

Emission of negative ions, positive ions and energetic neutral atoms from the lunar surface caused by solar wind precipitation 

Martin Wieser, Romain Canu-Blot, Stas Barabash, Aibing Zhang, Gabriella Stenberg-Wieser, and Wenjing Wang

A sizeable fraction of solar wind protons precipitating onto the lunar surface is backscattered from the lunar surface. Additionally the lunar surface is sputtered by the precipitating particle populations. Previous observations by spacecraft from orbit (Chandrayaan-1, Kaguya, IBEX) and from the lunar surface (Chang'e-4) show that up to 20% of the impinging solar wind protons are backscattered as energetic neutral atoms and about 0.1% to 1%  are backscattered as protons. However, particles emitted from the surface can have any charge state. The recent discovery of negative ions by the Negative Ions at the Lunar Surface (NILS) instrument on Chang'e-6 allows for the first time to investigate the full charge state distribution of solar wind induced backscattered and sputtered particle populations from the lunar surface. We present and interpret new data obtained from the lunar surface and discuss the impact of the emitted particle populations on the lunar exo-ionosphere.
 

How to cite: Wieser, M., Canu-Blot, R., Barabash, S., Zhang, A., Stenberg-Wieser, G., and Wang, W.: Emission of negative ions, positive ions and energetic neutral atoms from the lunar surface caused by solar wind precipitation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11607, https://doi.org/10.5194/egusphere-egu25-11607, 2025.

EGU25-12229 | Orals | PS1.3

Lunar Science With the HERMES Payload on Gateway 

William R. Paterson, Daniel J. Gershman, Shrikanth G. Kanekal, Roberto Livi, Mark B. Moldwin, Marilia Samara, Eftyhia Zesta, and Steven Christe

The Heliophysics Environmental and Radiation Measurement Experiment Suite, HERMES, is a science payload to observe electrically charged particles and magnetic fields from Gateway. Primary science goals include studies of the interplanetary medium and the terrestrial magnetosphere. The measurements will also be available and useful for studies of the lunar environment. The payload consists of an electron electrostatic analyzer, an ion mass spectrometer, an energetic ion and electron telescope, a set of magnetometers, and associated electronics. These instruments will be attached externally to Gateway’s Habitation and Logistics Outpost (HALO) prior to launch. The trip to lunar orbit will require approximately year, and the current Launch Readiness Date is not earlier than January 2027.  Gateway’s polar lunar orbit has a 4-week period, perilune altitude approximately 300 km above the north pole, and apolune at 70,00 km south. It is a sun-aligned halo orbit that will carry HERMES through the lunar wake once per month. The HERMES science mission begins after Gateway arrives at the moon and has nominal duration of 2 years. Although the project goals focus on heliophysics, the observations will have relevance for lunar science including studies of the exosphere and the structure and variability of the moon’s wake. The ion mass spectrometer will record the flux of terrestrial ions incident at the moon and pickup ions originating from the moon. Signatures of the Moon’s interaction with the space environment can be expected for all HERMES instruments. Data will be available to the public through Goddard Space Flight Center’s Space Weather SOC. With this presentation we discuss HERMES plans and capabilities with focus on science of the Moon.

How to cite: Paterson, W. R., Gershman, D. J., Kanekal, S. G., Livi, R., Moldwin, M. B., Samara, M., Zesta, E., and Christe, S.: Lunar Science With the HERMES Payload on Gateway, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12229, https://doi.org/10.5194/egusphere-egu25-12229, 2025.

EGU25-13081 | Posters on site | PS1.3

Exploring the origin of lunar magnetic anomalies through the Parker Inversion method 

Jacopo Baccarin, Joana S. Oliveira, Julia Maia, Bart Root, and Ana-Catalina Plesa

It is not yet understood whether the origin of the observed heterogeneous and weak lunar crustal magnetism is tied to a now extinct core-dynamo [1], to asteroid impacts [2, 3] or to a combination of both phenomena [4]. When using recent magnetic field maps (e.g., [5]) to study the magnetic sources, investigations to date have employed models relying on available geological and geophysical context, precluding the analysis of anomalies that are not correlated with known features. The Parker inversion method [6] overcomes these restrictions relying on a limited complexity of the magnetic sources by assuming unidirectional magnetization. It allows for the estimation of strength, location and direction of a set of surface dipoles that best fit the local set of magnetic data. We investigate the distribution of surface magnetization across the globe using Parker’s method independently of the specific geological or geophysical contexts, following the work of [7]. This approach enables the analysis of surface magnetic anomalies, ranging from those associated with impact craters (e.g., Moscoviense) or lunar swirls (e.g., Rimae Sirsalis) to the less-analysed polar regions. It captures varying morphologies, such as elongated (e.g., Hartwig), localized (e.g., Crozier), and more diffuse distributions (e.g., South Pole) of magnetized material. The overarching aim is to uncover the origin of magnetic anomalies and their significance for understanding lunar evolution.

Application of Parker’s method to isolated magnetic anomalies reveals a variety of magnetization distributions, reflecting the diversity of their morphologies and spatial patterns. Notably, a significant radial alignment of magnetized material related to the Imbrium basin suggests an ejecta origin for a number of near-side anomalies [2], for which the paleopole position is taken into consideration. We also see a clear correlation between the magnetization distribution and the antipodal regions of some large impact craters or basins, areas in which it is argued that the magnetic field could have been created or amplified by processes such as converging ejecta deposition, shock waves, and an ionized melt cloud from the impact [3, 4]. Finally, we recognize that the magnetized material of isolated and compact anomalies related to swirls aligns closely with the boundaries of these features [8], whereas large swirl structures show a poor correlation. This suggests the need for alternative analytical approaches for these regions.

Overall, our results reinforce previous hypotheses, in which large impacts played a pivotal role in shaping the morphology and distribution of lunar crustal magnetic sources.

 

References:

[1] Weiss B.P. and Tikoo S.M. (2014), Science (Vol. 346, Issue 6214)

[2] Hood L.L. et al. (2021), JGR Planets (Vol. 126, Issue 2)

[3] Hood & Artemieva (2008), Icarus (Vol. 193, Issue 2, pp. 485–502)

[4] Narrett et al. (2024), 55th LPSC

[5] Tsunakawa et al. (2015), JGR Planets (Vol. 120, Issue 6, pp. 1160–1185)

[6] Parker (1991), JGR Solid Earth (Vol. 96, Issue B10, pp. 16101–16112)

[7] Oliveira et al. (2024), JGR Planets (Vol. 129, Issue 2)

[8] Denevi et al. (2016), Icarus (Vol. 273, pp. 53–67)

How to cite: Baccarin, J., Oliveira, J. S., Maia, J., Root, B., and Plesa, A.-C.: Exploring the origin of lunar magnetic anomalies through the Parker Inversion method, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13081, https://doi.org/10.5194/egusphere-egu25-13081, 2025.

EGU25-13945 | Orals | PS1.3

Plasma on the lunar surface: Terra Incognita to be explored 

Stas Barabash, Yoshifumi Futaana, Philipp Wittmann, Thomas Maynadié, Akbar Whizin, and Angele Pontoni

To date, plasma observations on the lunar surface have been very limited. Most of these observations were conducted during the Apollo program, relying on technology that is now over 50 years old, or by a few individual sensors with narrowly defined scientific objectives on Chinese landers. Our knowledge of the plasma environment and the processes that govern it remains sparse, relying heavily on orbital measurements and theoretical models. This current level of understanding is insufficient to support the large-scale exploration efforts that are about to commence. In essence, we are navigating a "Terra Incognita" in this domain.

To characterize and understand near-surface plasma and its interactions with the lunar surface are required for:

  • Properly modeling surface and man-made object charging and potentials;
  • Investigating dust dynamics, including dust release and dust-plasma interactions;
  • Studying weathering processes that modify surface characteristics and compositions;
  • Establishing the role of the space environment in the formation, release, and dynamics of volatiles within the lunar exosphere;
  • Understanding plasma dynamics at the surface and interactions with various plasma domains as the Moon moves along the orbit.

Plasma and its interaction processes need to be studied across four fundamental scales:

  • Microscale (kinetic, 10-4 – 10-2 cm) to address microphysics of the particle – surface interaction
  • Mesoscale (sub-Debye, 10 cm–10 m) to investigate plasma process when quasi-neutrality breaks creating strong electric fields
  • Macroscale (MHD, 10 m–1 km) to explore connections between plasma dynamics and topography
  • Global scale (MHD, 1 km–1,000 km) to reveal effects of large-scale structures, such as magnetic anomalies and the terminator, on local plasma populations.

In this presentation, we demonstrate the limitations of our current knowledge, highlight the critical importance of advancing it, and outline steps to explore the "Terra Incognita" of plasma on the lunar surface.

 

How to cite: Barabash, S., Futaana, Y., Wittmann, P., Maynadié, T., Whizin, A., and Pontoni, A.: Plasma on the lunar surface: Terra Incognita to be explored, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13945, https://doi.org/10.5194/egusphere-egu25-13945, 2025.

EGU25-14271 | Posters on site | PS1.3

Mineralogical and Geochemical Study of the Low-Ti Lunar Basaltic Meteorite NWA_16727 

Yiyi Ban, Xiaochao Che, Cheng Yue, Tao Long, and Dunyi Liu

NWA_16727 is a lunar basaltic meteorite recovered from Northwest Africa, characterized by a medium-grained subophitic texture. The primary mineral assemblage consists of pyroxene and maskelynite with small amounts of olivine, chromite, ilmenite, phosphate, silica, Fe-Ni metal, and zircon-rich phases. Pyroxene appears as subhedral to anhedral grains, typically medium-grained. These grains exhibit strong compositional zoning from Mg-rich cores to Fe-rich rims, with Fe/Mn ratios ranging from 47 to 98. Measured Fe# varies between 0.33–0.99, and Mg# varies between 0.50 and 66.9, values consistent with known lunar basalts. Fractures are common, and some grains contain melt pockets. Olivine crystals are zoned grains featuring Mg-rich cores that transition to Fe-rich rims (Fo~6–63), commonly hosting melt inclusions. These compositional differences produce a bimodal olivine population at Fa36–65 and Fa70–95, with Fe/Mn ratios of 93–141. Surfaces often show fractures resembling shock-induced features observed in other lunar materials. Raman spectroscopy confirms that plagioclase has been entirely transformed to maskelynite in most instances, demonstrating high-pressure shock metamorphism. Typical compositions range from An85–91 to Or0.17–0.76. Maskelynite grains remain relatively clear surface, although microfractures cross-cut certain regions, suggesting extensive shock deformation. Abundant mineral fragments, impact melt veins, and shock-induced glass are observed throughout the sample. Impact melt veins incorporate partially melted pyroxene, silica, glassy melt, and nanometer-scale Fe-metal and troilite. Ilmenite and chromite constitute the main Fe-oxides, typically forming euhedral to subhedral grains associated with pyroxene or olivine. Aggregates of olivine and Cr-Ti-Fe spinels are often rimmed by Fe-rich reaction zones. Fe/Mn ratios in pyroxene and olivine confirm the sample’s lunar origin. Pyroxene Ti/(Ti+Cr) and ratios are comparable to those found in low-Ti basalt groups. Rare Earth Element patterns, normalized to CI chondrites, highlight a negative Eu anomaly in pyroxene, alongside relative depletion of both light and heavy REE. Conversely, plagioclase shows strong LREE enrichment and a significant positive Eu anomaly. Overall, the meteorite is classified as a low-Ti basalt. Its pyroxene compositions closely resemble those of other lunar basalts, especially NWA14526, NWA_13137, and NWA_12008, and the pyroxene and maskelynite REE pattern align well with NWA_12008. Based on comprehensive petrological, mineralogical, and geochemical evidence, we hypothesize that NWA_16727 and NWA_12008 may represent paired meteorites.

How to cite: Ban, Y., Che, X., Yue, C., Long, T., and Liu, D.: Mineralogical and Geochemical Study of the Low-Ti Lunar Basaltic Meteorite NWA_16727, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14271, https://doi.org/10.5194/egusphere-egu25-14271, 2025.

EGU25-14967 | Posters on site | PS1.3

The Terrain Testing Instrument (TTI) as a Selected Payload for the Chang'e 8 Lunar Landing Mission 

Lutz Richter, Meng Zou, and Bernard Foing

This contribution describes the so-called Terrain Testing Instrument (TTI) which has recently been selected as an international payload for the planned Chinese Chang’e 8 lunar landing and roving mission targeting a high southern latitude landing site. The TTI will measure lunar regolith penetration resistance and shear strength, in a so-called vane-cone instrument that combines a cone penetrometer and a shear vane. A permittivity sensor using a novel patch electrode arrangement is integrated with the vane-cone and will allow to infer bulk density and ice content of the regolith, derived from measurement of the dielectric properties such as relative permittivity.

In the initial phase of lunar surface exploration by the United States and the Soviet Union, dedicated instruments were designed and used to measure in situ some key physical properties of the regolith column in various locations. On the lunar landing and roving missions of the modern era however, no instruments have yet been flown for such purposes. It will however be particularly important to understand regolith stress-strain behavior in the South polar region as well as local volatiles contents, as extensive landing, roving, mining, and construction activities are foreseen there over the next several decades. A general assumption is that regolith in the South polar area would broadly resemble lunar highland regolith. But direct measurements will be indispensable ahead of crewed missions.

Volatiles constitute an important resource while at the same time sublimation of ices from an icy regolith in response to loading and thermal dissipation from human-emplaced structures can lead to subsistence of the ground, thus constituting a hazard. The TTI will address these critical gaps in knowledge.

The TTI is a slender penetrometer with a frontal shear vane for quasi-static regolith intrusion. A linear translation mechanism will drive it into the regolith while resistance vs. depth is recorded, followed by rotation of the shear vane to indicate shear resistance as a function of shear angle. Depth range of the TTI instrument is ~10…20 cm. It will be carried on a mobile rover and perform multiple measurement runs during the Chang’e 8 mission at various locations, thanks to the mobility of the carrying platform. The TTI overall mass is ~1.5 kg. The instrument is being developed by an international team of entities from Germany, the Netherlands, and China.

How to cite: Richter, L., Zou, M., and Foing, B.: The Terrain Testing Instrument (TTI) as a Selected Payload for the Chang'e 8 Lunar Landing Mission, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14967, https://doi.org/10.5194/egusphere-egu25-14967, 2025.

EGU25-15674 | ECS | Orals | PS1.3 | Highlight

Lunar volcanism: A Geophysical perspective 

Adrien Broquet, Jeff C. Andrews-Hanna, and Ana-Catalina Plesa

The lunar crust has preserved a record of the Moon’s volcanic and magmatic activity through time. While the extrusive maria dominate the volcanic record, little is known regarding their thickness and the details of their emplacement. Intrusive activity is even more elusive, with most intrusions expressing little to no surface signature. Here, we present a global investigation and a volumetric inventory of extrusive and intrusive volcanic materials (Broquet & Andrews-Hanna, 2024a, 2024b). Gravity and topography are inverted using a two-layer loading model under the premise of pre-mare isostasy to constrain mare and cryptomare thickness, as well as updated crustal thickness models. Substantial lateral variations in mare thickness are found, with averages 7.9 km within large mare basins compared to 1.6 km outside of these basins. This important thickness variation associated with minimal change in the surface topography can be explained by some combination of long-distance transport of low viscosity mare and/or a buoyancy control limiting mare eruptions to a constant level surface.

Our inversion predicts the shape of the lunar crust before it got obscured by mare materials. The pre-mare surface of the nearside Oceanus Procellarum region is ~2 km lower than the surroundings, and possible explanations, including a giant impact, pore space annealing, isostatic adjustment, and plume-induced crustal erosion, are discussed. The western part of Imbrium’s ring is not found in the pre-mare topography, implying that it never formed or that some processes erased its signature from gravity and topography. The feldspathic, pre-mare, crust is ~7 km thinner within large nearside basins than in models not accounting for the high-density mare. The pre-fill floor of these basins was ~6 km deeper than currently observed. These new insights have implications for impact simulations that try to reproduce the crustal structure of nearside mare basins.

Our preferred volumes of mare and cryptomare total to 20×106 km3. Investigation of crustal intrusions associated with linear gravity anomalies, floor-fractured craters, ring dikes, graben, and beneath volcanic constructs, yield a total volume of 9×106 km3. The major fraction of intrusive materials is in the form of ring dikes located at the margin of large basins in zones of flexural extension, which indicates an important control of lithospheric stress on magma ascent. Taken together, the total volume of the secondary crust corresponds to ~2% (and up to 5%), of the total lunar crust volume. The combined volume of intrusives and extrusives is found to be 3 times greater in the nearside than in the farside. Intrusive activity dominates in the farside (intrusive:extrusive ratio of 5:2), whereas extrusive volcanism is more pronounced in the nearside (1:5). Both are related to the lunar asymmetry in which the thinner crust and warmer subsurface beneath the Procellarum KREEP terrane enables enhanced melting and magma ascent. The strong asymmetry in melt production supports an early KREEP migration, which must have been established 100 s of Myr before nearside volcanism began to allow for the buildup of heat.

 

Broquet, A., & Andrews-Hanna, J.C. (2024a). Icarus 408. 10.1016/j.icarus.2023.115846.

Broquet, A., & Andrews-Hanna, J.C. (2024b). Icarus 411. 10.1016/j.icarus.2024.115954.

How to cite: Broquet, A., Andrews-Hanna, J. C., and Plesa, A.-C.: Lunar volcanism: A Geophysical perspective, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15674, https://doi.org/10.5194/egusphere-egu25-15674, 2025.

EGU25-16581 | ECS | Orals | PS1.3

Visiting the emptiest space – Analysing the JUICE Lunar flyby PEP-JDC data  

Philipp Wittmann, Martin Wieser, Stas Barabash, Gabriella Stenberg Wieser, Thomas Maynadié, Norbert Krupp, Elias Roussos, Markus Fränz, Pontus Brandt, Peter Wurz, Jasper Halekas, and Andrew Poppe and the PEP Team

The JUpiter ICy moons Explorer (JUICE) performed end of August 2024 its Lunar-Earth gravity assist consisting of a flyby of the Moon followed by an Earth flyby. During this manoeuvre the Particle Environment Package (PEP) was operated to investigate both the near lunar and the magnetospheric environment and to validate its performance. PEP consists of six individual sensors detecting ions, electrons and ENAs depending on their energy, arrival direction and mass. Here we focus on measurements of one of these sensors, the Jovian plasma Dynamics and Composition analyzer (JDC). JDC measures angular and mass-resolved positive and negative ions as well as electrons in an energy range from a few eV/q up to 35 keV/q. The JDC field of view covers a hemisphere and is divided into 16 x 12 angular pixels.

We present JDC data from the lunar flyby. During the flyby, the Moon was in Earth’s magnetotail. JUICE approached the moon from the side of the lunar wake. JDC was operated for ~103 minutes during the flyby with the exception of an 8 minutes long period around the closest approach to the Moon. The observed plasma densities during the lunar flyby were extremely low - making this region one of the emptiest spaces. Nevertheless, after entering the lunar optical shadow until the end of the measurement interval a weak signal at ~1.5 keV/q was detected. This signal is not an instrument background and is not visible before entering the Lunar optical shadow. We show ray tracing results to investigate the possible origin of these particles.

How to cite: Wittmann, P., Wieser, M., Barabash, S., Stenberg Wieser, G., Maynadié, T., Krupp, N., Roussos, E., Fränz, M., Brandt, P., Wurz, P., Halekas, J., and Poppe, A. and the PEP Team: Visiting the emptiest space – Analysing the JUICE Lunar flyby PEP-JDC data , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16581, https://doi.org/10.5194/egusphere-egu25-16581, 2025.

EGU25-19008 * | Orals | PS1.3 | Highlight

First campaigns and future developments in the LUNA Moon analog facility 

Martin Knapmeyer, Brigitte Knapmeyer-Endrun, Michael Maibaum, Cinzia Fantinati, Maria Hallinger, Oliver Küchemann, Christos Vrettos, Dirk Plettemeier, Wolf-Stefan Benedix, Titus Maria Casademont, Jan Seeling, Jörg Knollenberg, Johannes Hart, Laura Alejandra Pinzon Rincon, Philippe Jousset, Charlotte Krawczyk, Raphael F. Garcia, Lapo Calosci, and Carl Spichal

The current renaissance in lunar exploration, driven by space agencies as well as the private sector, requires suitable test and training facilities on Earth to proceed in a safe and sustainable manner. To address this need, DLR and ESA have opened the Moon analogue facility LUNA in Cologne, Germany, in September 2024. We will provide an overview of LUNA and report on first campaigns, which already included usage by universities, national space agencies, and the private sector.

At the heart of LUNA is a 700 m² regolith hall, filled with Mare simulant EAC-1A to 60 cm depth. With black walls, a preliminary sun simulator allowing to simulate illumination at the lunar south polar region, geologically relevant rocks, an Argonaut lunar lander mock-up, two 3U-rovers that might carry individual instruments, and a future gravity offloading, LUNA simulates the lunar surface and allows to test the operations of instruments and experiments on the Moon as well as train operations for robotic and crewed lunar missions. A dedicated ground segment permits commanding and telemetry and data exchange under mission-like conditions. Further outfitting by elements both within (e.g. a ramp to simulate slopes of at least up to 40 deg) and outside of LUNA (e.g. Flexhab habitat, EDEN-LUNA greenhouse) is ongoing.

The deep floor area (DFA), with a regolith depth of up to 3 m over an area of approximately 135m² and two sloping walls with angles of 25° and 40°, allows for testing geophysical exploration methods as well as drilling and sampling techniques. The initial outfitting of the DFA includes two buried metal reference targets for ground-penetrating radar (GPR), as well as a small simulated lava tunnel at the bottom, constructed from concrete and expanded foam sheets. Additionally, PMMA (aka Plexiglas™) is used to simulate the elastic and dielectric contrasts between regolith and ice, which is of special interest in exploration of the lunar South Pole, and emplaced to mimic both a thin ice horizon as well as distributed veins of ice (reticular chaotic cryostructure, formed by 1000 PMMA discs). A fiber-optic cable, including fibers for distributed temperature sensing (DTS), distributed acoustic sensing (DAS), and an engineered fiber, has been buried throughout the hall to be used for background data, and a broad-band seismometer has been installed permanently in LUNA. Several seismic reference measurements as well as a GPR test have been conducted to characterize the LUNA hall and environment.

The EAC-1A simulant has been characterized in terms of elastic, electric and thermal properties, e.g. seismic wave velocities and attenuation from resonant column tests, dielectric permittivity and loss tangent, and thermal conductivity. We show in how far these parameters match the values for actual lunar regolith. We will also report on first test campaigns, e.g. regarding geophones and the engineered DAS fibre, GPR, and rover navigation.

How to cite: Knapmeyer, M., Knapmeyer-Endrun, B., Maibaum, M., Fantinati, C., Hallinger, M., Küchemann, O., Vrettos, C., Plettemeier, D., Benedix, W.-S., Casademont, T. M., Seeling, J., Knollenberg, J., Hart, J., Pinzon Rincon, L. A., Jousset, P., Krawczyk, C., Garcia, R. F., Calosci, L., and Spichal, C.: First campaigns and future developments in the LUNA Moon analog facility, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19008, https://doi.org/10.5194/egusphere-egu25-19008, 2025.

The nature of the sources and processes involved in the formation of Lunar High-Al and High-Ti basalts are not completely understood. Through petrological experiments designed to study the effects of inefficient plagioclase flotation during late-stage Lunar Magma Ocean (LMO) crystallization, we were able to find a possible mechanism for the Al and Ti enrichment for both types of basalts. Retained plagioclase in late-stage ilmenite-bearing cumulates (IBCs) within the lunar mantle results in low-fraction (1-10%) partial melts that are highly enriched in Al and have a high affinity with the composition of Apollo 14 and Luna 16 high-Al basalts. Additionally, melting of Ti-rich phases ilmenite and ülvospinel, is prominent at higher partial melting fractions (20-60%) resulting in melts that can be enriched in over 20% TiO2, with high affinity to high-Ti basalts and picritic glasses.

These results imply that both types of magmas may share the same mantle source but formed at different stages of fractional melting processes. The ages of both basalt types may be related to this fractional melting process, with high-Al basalts known to be the oldest Lunar volcanism and youngest known samples, overlapping with the oldest ages for high-Ti basalts at ~3.8 Ga. Our findings can explain multiple aspects of the major element composition of these basalts, but there are other aspects that need to be accounted for. The higher-than-expected Mg contents in both types of basalts, and the presence of olivine and orthopyroxene in the multiple saturation points of high-Ti basalts despite the absence of these minerals in IBCs, indicate that additional processes are involved in the formation of these basalts or even in the formation of mantle cumulates.

The inefficient flotation of plagioclase during LMO crystallization has been proposed as a possible explanation for the lower thickness of the lunar crust compared to experimental determinations [1]. Our findings provide further evidence that flotation inefficiency is a possibility, and its consequences may go beyond crustal thicknesses, but may also affect posterior mantle dynamics and the composition of lunar volcanism.

[1] Charlier, B. et al. (2018), Geochim. Cosmochim. Acta. 234, 50-69.

How to cite: Astudillo Manosalva, D. and Elardo, S. M.: Inefficient plagioclase segregation during Lunar Magma Ocean Crystallization can link the mantle sources for High-Alumina and High-Titanium basalts, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19115, https://doi.org/10.5194/egusphere-egu25-19115, 2025.

EGU25-20197 | ECS | Orals | PS1.3

Legacies and Lessons: Learning from Apollo 16 and 17 sampling for future autonomous planetary exploration 

Divya M Persaud, Cynthia B Phillips, and Kevin P Hand

In planetary exploration, once a landing site has been selected and a mission has successfully landed, one of the next decisions will be sampling location. Stationary missions that do not have the benefit of mobility, such as pathfinding landers to ocean worlds like Europa, and those limited by surface lifetime, will require some degree of autonomy in the selection of sampling locations within a reachable workspace (Hand et al., 2022). Therefore, the process of sample location selection is worth constraining.

In this work, we investigate Apollo 16 and 17 sampling sites, treating the Moon as our best Europa analogue. We use archival reports, imagery, and other data of four Apollo 16 and three Apollo 17 sites and their corresponding drive tube core samples to constrain how the surface appearance of sampling sites couples with subsurface geology. The surface and subsurface geology are summarized using bin classifications for grain size and shape as first-order representations of regolith formation processes, and then compared with each other and contextualized by descriptions of the astronauts’ sampling decision-making to understand the impact factors in sampling the surfaces of worlds like the Moon. The work is relevant to other data-constrained, short-lived surface sampling missions that will rely on autonomy, as well as future human sampling activities during crewed exploration (e.g., the Artemis program).

References

Hand, K. P., C. B. Phillips, A. Murray, J. B. Garvin, E. H. Maize, R. G. Gibbs, G. Reeves, et al. 2022. “Science Goals and Mission Architecture of the Europa Lander Mission Concept.” The Planetary Science Journal 3 (1): 22. https://doi.org/10.3847/psj/ac4493.

How to cite: Persaud, D. M., Phillips, C. B., and Hand, K. P.: Legacies and Lessons: Learning from Apollo 16 and 17 sampling for future autonomous planetary exploration, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20197, https://doi.org/10.5194/egusphere-egu25-20197, 2025.

EGU25-20532 | Orals | PS1.3

Variations in Lunar Crater Populations Due to Target Properties 

Jean-Pierre Williams, Asmin Pathare, and Emily Costello

Crater chronology models rely on correlating observed crater size-frequency distributions (CSFDs) on the ejecta blankets of Copernican-age craters with cosmic-ray exposure ages of samples acquired by Apollo missions. However, these crater populations are known to vary on the ejecta of these craters. One explanation is that impact melts, boulders, and other variations in material properties can influence the scaling of impact craters. We conduct crater counts on the ejecta of several Copernican-age craters and find that crater densities vary with the thermophysical properties of the ejecta as observed by the Lunar Reconnaissance Orbiter Diviner instrument, providing evidence that the strength of ejecta materials can have a significant influence on CSFDs. Specifically, we find that as Diviner-derived rock abundance increases, the spatial density of craters decrease. Absolute model ages are affected as areas of higher rock abundance yield younger ages. This suggests terrain properties should be taken into consideration when deriving absolute model ages.

How to cite: Williams, J.-P., Pathare, A., and Costello, E.: Variations in Lunar Crater Populations Due to Target Properties, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20532, https://doi.org/10.5194/egusphere-egu25-20532, 2025.

EGU25-20732 | Posters on site | PS1.3

The Miniaturized Electron Proton Telescope on board HERMES 

Shrikanth G Kanekal

The Lunar Gateway, part of NASA’s Artemis program, is a space station orbiting around the moon expected to launch in 2027. The Heliophysics Environmental and Radiation Measurement Experiment Suite (HERMES) is a suite of instruments placed on the outside of the Habitation and Logistics Outpost (HALO)  to study the coupled Sun-Earth system and monitor the Sun’s radiation environment and space weather.

We describe in detail the  Miniaturized Electron Proton Telescope (MERiT) on board HERMES. MERiT  measures electrons and protons in the energy range ~0.5-9.0 MeV and ~1-190 MeV in 11 and 20 differential energy channels respectively. MERiT is a solid-state detector telescope with the two sensor heads facing sunward and  anti-sunward directions. MERiT will study solar energetic particles, low energy cosmic rays and energetic electrons in the magnetospheric tail. 

The MERiT has also been proposed to the ARTEMIS Lunar Terrain Vehicle program. On the Lunar surface, MERIT will characterize charged particle effects on the regolith, probe for sub-surface hydration, explore micro magnetization and study dielectric discharge effects due to penetrating cosmic rays, and high energy solar protons.

How to cite: Kanekal, S. G.: The Miniaturized Electron Proton Telescope on board HERMES, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20732, https://doi.org/10.5194/egusphere-egu25-20732, 2025.

EGU25-21276 | Posters on site | PS1.3

  Identification of a lunar volcanic dome termed L1 in Promontorium Laplace and mineralogy 

Maximilian Teodorescu and Raffaello Lena

In recent years, with the advancements in digital sensors technology and access to space probes data, more and more lunar features are discovered using ground-based images. Mostly, these features are lunar domes, with tens of such structures being discovered using medium-sized telescopes.

In the following study we examine a lunar dome, termed Laplace 1 (L1), identified using telescopic images, Lunar Reconnaissance Orbiter (LRO) Wide Area Camera (WAC) images, the Laser Altimeter Digital Elevation Model (LOLA DEM), and the LRO WAC-based GLD100 Digital Terrain Model (DTM) along with data from the Chandrayaan-1 Moon Mineralogy Mapper, Diviner dataset and Kaguya Multiband Imager. The dome lies at coordinates of 48.57°N and 26.37°W, at about 36 km south east of the crater Maupertuis, and has a base diameter of 7.6 km ± 0.3 km, a maximum height of 230 ± 20 m, resulting in a slope angle of 3.4° ± 0.3°. We also infer the mineralogical composition of the dome.

 

How to cite: Teodorescu, M. and Lena, R.:   Identification of a lunar volcanic dome termed L1 in Promontorium Laplace and mineralogy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21276, https://doi.org/10.5194/egusphere-egu25-21276, 2025.

EGU25-552 | ECS | Posters on site | PS7.2

Spatio-Temporal Analysis of Phase Change Material Based Heat Accumulator Under Space and Planetary Environment 

Keyur Kansara, Shobhana Singh, Navin Kumar Dwivedi, and Maxim L. Khodachenko

Phase Change Materials (PCMs) are increasingly recognized for their potential in effective thermal management of space systems. PCM based heat accumulators maintain the temperature stability of electronic payloads in Spacecraft, Orbiters, and Landers, ensuring their reliability during operations. The primary challenge lies in understanding the complex convection dynamics that occurs during the solid-liquid phase transition. Key factors influencing the phase change dynamics in a space or planetary environment include the absence of atmospheric pressure, variations in incident heat flux, and low or varying gravitational acceleration. Under such conditions, the imbalance between convective and diffusive heat fluxes during the solid-liquid phase change leads to complex morphologies at the phase interface, which interfere with the effectiveness of heat transfer through the accumulator. In this study, we investigate the influence of variable gravity and its relative orientation with the global temperature gradient, defined by angle α, on the performance of the PCM-based heat accumulator. We study the spatio-temporal changes in flow dynamics across the orientation angle range from 0° to 180°, where, α = 180° corresponds to the alignment of the incoming heat flux with the gravity field, and α = 0° depicts the configuration where they are oriented in opposite direction. We conduct statistical analysis of coherent structures and global heat transport characteristics to examine the influence of variable gravitational conditions and orientation angles on the flow dynamics, heat transport, and thus the overall melting process of PCM. In addition, the variation in the energy storage capacity of PCM is provided under different operational conditions, which contributes to our understanding of the requirements for PCM in the design of thermal management systems for spacecraft.  The results are vital in assessing and designing a PCM-based heat accumulator for long-term passive thermal control in space and planetary environments.

How to cite: Kansara, K., Singh, S., Dwivedi, N. K., and Khodachenko, M. L.: Spatio-Temporal Analysis of Phase Change Material Based Heat Accumulator Under Space and Planetary Environment, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-552, https://doi.org/10.5194/egusphere-egu25-552, 2025.

We propose an instrument, MsRAIN designed to investigate the feasibility of creating artificial rain outside Earth and in low gravity conditions. MsRAIN is the second generation of instruments, where the first generation was tested onboard the International Space Station (ISS) in May 2023 through the Saudi Space Agency (SSA) Cloud Seeding in Microgravity Experiment. MsRAIN is designed to work in future human colonies on the Moon and Mars as it can help in having a better spatial distribution of water on the colonies. 
MsRAIN is composed of four hydrophobic chambers each containing an air pump, small water container, humidifier, silver iodide container, meteorological sensors, power supply, and high-speed cameras. 
The core perspective in MsRAIN is that physical experiments are needed to understand the possibility of artificial rain formation on the Moon and Mars. Little is known about the behavior of condensation of water vapor on aerosol particles in reduced (fractional) gravity environments (less than the nominal 1 g that occurs on Earth). 
On Earth, cloud seeding missions are widely used in many countries to enhance the amount of precipitation in rain scarcity regions, however, the seeding agents (silver iodide for example) sprayed in the air can be affected by the Earth’s gravity and fall to the ground and to the water bodies which can affect the environment. The lower gravity conditions on the Moon and Mars could help seeding agents stay longer in the atmosphere (if any), consequently providing a better chance for the formation of water droplets. 
The MsRAIN payload team is led by mid-career scientists, engineers, graduate, and undergraduate students from different research institutes in Saudi Arabia. The team includes SSA and the King Fahd University of Petroleum and Minerals (KFUPM).

How to cite: Farahat, A. and Smith, H.: Examining MsRain for the Possibility of Creating Artificial Rain with Cloud Seeding Techniques on the Moon and Mars Future Human Settlements , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1412, https://doi.org/10.5194/egusphere-egu25-1412, 2025.

EGU25-2166 | Posters on site | PS7.2

Data archive for EDI instrument on Cluster spacecrafts: measurements and data processing 

Mikhail Rashev and Patrick Daly

The Electron Drift Instrument(EDI) onboard of four Cluster spacecrafts measures electric filed E in the near Earth orbit. By measuring a drift of 1keV electrons the instrument determines the value of the electric field E in the plane perpendicular to the magnetic field B.

The Cluster mission life-time is more then 20 years. Over this time the EDI provides data for electric field, drift velocity, electron counts. Data are provided with various time intervals from milliseconds to 4seconds. Therefore it is possible to track fast changes in boundaries.

Instrument teams collect data, extracts physical values from raw data, calibrate them and deliver these values as data products to ESA central archive.

Once the instrument is in space many aspects of data handling become routines and can be automated. In the last decade the industrial big data segment produced many tools that can be used to automate scientific data processing.

How to cite: Rashev, M. and Daly, P.: Data archive for EDI instrument on Cluster spacecrafts: measurements and data processing, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2166, https://doi.org/10.5194/egusphere-egu25-2166, 2025.

EGU25-2924 | Orals | PS7.2

The Europa Clipper Gravity and Radio Science (G/RS) Investigation 

Erwan Mazarico, Dustin Buccino, Julie Castillo-Rogez, Andrew Dombard, Antonio Genova, Hauke Hussmann, Walter Kiefer, Jonathan Lunine, William McKinnon, Francis Nimmo, Ryan Park, James Roberts, Paolo Tortora, and Paul Withers and the Europa Clipper G/RS Team

NASA’s Europa Clipper flagship mission launched on October 14, 2024 and will arrive at Jupiter in April 2030. There, it will investigate the habitability of Jupiter’s moon Europa. Gravity and Radio Science (G/RS) is one of ten complementary investigations devoted to understanding Europa through studies of its ice shell and ocean, its composition, and its geology. G/RS makes use of the Europa Clipper telecommunications system to obtain radiometric tracking data during the Europa flybys.

Unlike past missions, the primary raw data for the G/RS investigation are obtained from Open-Loop Receivers (OLR) at the Deep Space Network (DSN) ground stations. Indeed, the flyby geometry, spacecraft attitude, and spacecraft antenna configuration are such that the signal-to-noise ratio of the return radio signals will be small (<10 dB-Hz) and insufficient for the typical closed-loop tracking. Processing of the OLR with special retracking algorithms will be necessary to obtain range-rate (Doppler) observations. Given the lack of a stable oscillator onboard Europa Clipper, two-way tracking will be used to achieve high frequency stability, leveraging the accurate DSN clocks. Radio tracking during the flybys will be performed at a single frequency (X-band), so careful modeling of media perturbations is important to maximize the G/RS results. We will discuss recent work to assess the impact of media perturbations from the Io Plasma Torus on orbit reconstruction and geophysical parameter recovery.

G/RS will obtain measurements of Europa’s static and time-variable gravity field.  The tidal Love number k2 will verify the presence of a subsurface ocean and help constrain the ice shell. The moment of inertia, derived from degree-2 gravity coefficients, will help determine the interior structure. The radio tracking data will also be sensitive to Europa’s ionosphere when geometry allows.

We will present the G/RS investigation and observation plans, its expected performance, and provide a first look at the tracking data during cruise.

How to cite: Mazarico, E., Buccino, D., Castillo-Rogez, J., Dombard, A., Genova, A., Hussmann, H., Kiefer, W., Lunine, J., McKinnon, W., Nimmo, F., Park, R., Roberts, J., Tortora, P., and Withers, P. and the Europa Clipper G/RS Team: The Europa Clipper Gravity and Radio Science (G/RS) Investigation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2924, https://doi.org/10.5194/egusphere-egu25-2924, 2025.

EGU25-4073 | Orals | PS7.2

PREMIER - Plasma Brake Multi-target Active Debris Removal Mission for Low Earth Orbit 

Maria Genzer, Pekka Janhunen, Harri Haukka, Olli Knuuttila, Leo Nyman, Antti Kestilä, Perttu Yli-Opas, Kari Mäkiniemi, Miguel Olivares Mendez, Carol Martinez Luna, Abishek Bera, Fabrizio Scarpa, Angelo Maligno, Marius Klimavicius, and Tomas Malinauskas

We are proposing a mission concept for Active Debris Removal (ADR) of multiple uncooperative debris targets from Low Earth Orbit, using a minisat spacecraft ("mothership") carrying several Coulomb Drag based Plasma Brake¹ modules. The Plasma Brake technology enables very high downmass/upmass ratios for debris deorbiting. In optimal conditions, the ratio for such a mission could be up to 60, representing a radical increase in ADR performance of 1-2 orders of magnitude compared to the current state-of-the-art ADR missions, and drastically improving the cost efficiency compared to one-object-per-mission approaches. The  Plasma Brake is especially competitive in the ~700-1200 km altitude range. The applicable debris mass limit of this deorbiting method is dictated by the demisability of the targets and is roughly 500 kg / Plasma brake unit. It provides a scalable, cost-effective method for reaching a net-zero space debris operations in the long term.

The mission scenario consists of transfers between targets and a sequence of mothership operations repeated at each target: rendezvouz, detection, approach, de-tumbling of the target, attachment of a Plasma Brake module to the target. The critical core technologies needed to realize the mission, and are currently at low TRL, include:

  • Sensors, actuators and algorithms required for the proximity operations used to approach and de-tumble the target object,
  • Capture/attachment technologies for uncooperative targets like: kinematic structures, Hoberman sphere mechanisms, electrostatic adhesive,
  • Adaptation of Plasma Brake concept to work with uncooperative targets,
  • Framework for choosing the targets of a a multi-object touring mission that maximizes the downmass/upmass ratio, including the navigation scheme and navigation algorithms.

Most ADR technologies so far are only viable for deorbiting large pieces of debris. The proposed system allows the effective deorbiting of much smaller pieces of debris as well, maintaining its effectiveness indefinitely to clean up the debris that is required by zero-debris targets.

The mission concept and development of the critical core technologies needed for the mission to TRL 4 (testing prototypes in laboratory environment) have been proposed in EIC Pathfinder call of October 2024 by the authors.

¹Janhunen, P., Electrostatic plasma brake for deorbiting a satellite, J. Prop. Power, 26, 370-372, 2010, https://arc.aiaa.org/doi/10.2514/1.47537

How to cite: Genzer, M., Janhunen, P., Haukka, H., Knuuttila, O., Nyman, L., Kestilä, A., Yli-Opas, P., Mäkiniemi, K., Olivares Mendez, M., Martinez Luna, C., Bera, A., Scarpa, F., Maligno, A., Klimavicius, M., and Malinauskas, T.: PREMIER - Plasma Brake Multi-target Active Debris Removal Mission for Low Earth Orbit, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4073, https://doi.org/10.5194/egusphere-egu25-4073, 2025.

EGU25-4088 | Posters on site | PS7.2

Trajectory calculations problematics with the Earth atmosphere entering bodies and FSSAC probabilistic solution approach 

Harri Haukka, Leo Nyman, Ari-Matti Harri, Antti Kestilä, Maria Genzer, Petri Koskimaa, Olli Knuutila, and Iina Jaakonaho

Study Problematics

Space situational awareness (SSA) main object is to produce as real-time an overall picture of the space situation as possible. By developing abilities, methods and models to observe objects and bodies located in near Earth space and by predicting space weather phenomena, the risks of damage to both people and property caused using space can be reduced.

In this study discussion we focus into problematics that we have especially with the final phase trajectory calculations for space debris, deorbiting satellites and other bodies. Despite we can know the orbits of the satellites or debris very well, the final atmospheric entry determination is challenging. This challenge will be discussed and the main elements of future improvements that should be developed to reach more precise determination capabilities will be introduced. The main problematics to predict the atmospheric entering bodies (manmade and natural) can summarized to following focus areas:

  • Earth atmosphere is not perfect circle in real life. Space weather events cause significant changes in the upper atmosphere composition and altitude [1] [2]. 
  • Satellites aren’t optimal nor unified in shape and satellite mass is not really known. Satellite models for de-orbiting calculations simplifies [3] the shape and surface area of the satellite.
  • The velocity of the satellite is high and hard to follow in the end and angle of attack of the atmospheric re-entry is unclear. 

FSSAC Probabilistic Solution Approach

The Finnish Space Situational Awareness Center (FSSAC) is developing systems to estimate the impact areas and effects of space objects entering Earth’s atmosphere. Accurate orbital parameters are critical for determining impact points [4], but publicly available data, such as TLEs processed with the SGP4/SDP4 model, lack precision. These datasets are updated infrequently and exclude certain objects, such as military satellites.

To address this, FSSAC integrates additional data like covariance matrices, SGP4-XP, CPF, and Sp3c products, alongside Satellite Laser Ranging (SLR) data. The Metsähovi SLR telescope is being upgraded with a new laser emitter to expand coverage of RSOs, enhancing orbit modeling accuracy. Reliable atmospheric models are also essential, but existing options, such as NRLMSISE‐00 [5], are outdated and can produce errors of 20–30% during high solar activity.

FSSAC is advancing atmospheric models and orbit propagation tools to support accurate re-entry predictions. These efforts aim to provide timely warnings for high-risk RSOs, prioritizing public safety.

References
[1] https://www.ilmatieteenlaitos.fi/ajankohtaista/1244013

[2] Baruah, Y., et.al. (2024). “The loss of Starlink satellites in February 2022: How moderate geomagnetic storms can adversely affect assets in low-earth orbit”. Space Weather, 22, e2023SW003716. https://doi.org/10.1029/2023SW003716

[3] https://sdup.esoc.esa.int/

[4] Pardini, Carmen, and Luciano Anselmo. "Overview of some basic requirements for a reentry prediction service for civil protection applications." Proc. 1st NEO and Debris Detection Conference, Darmstadt, Germany. 2019.

[5] Picone, J. M., et al. ”NRLMSISE-00 empirical model of the atmosphere: Statistical comparisons and scientific issues”, JGR Volume107, IssueA12, 2002, https://doi.org/10.1029/2002JA009430

How to cite: Haukka, H., Nyman, L., Harri, A.-M., Kestilä, A., Genzer, M., Koskimaa, P., Knuutila, O., and Jaakonaho, I.: Trajectory calculations problematics with the Earth atmosphere entering bodies and FSSAC probabilistic solution approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4088, https://doi.org/10.5194/egusphere-egu25-4088, 2025.

EGU25-4996 | ECS | Orals | PS7.2

The Next-Generation Life Marker Chip: A Photonic Biosensor for Space Exploration 

Niels Frank Willem Ligterink

Building upon the heritage of the Life Marker Chip (LMC) developed for Mars exploration (Sims et al. 2012), I present an advanced integrated photonic biosensor for in-situ molecular detection in space environments. The system employs an asymmetric Mach-Zehnder Interferometer (aMZI) fabricated using silicon nitride waveguide technology, enabling label-free detection of biomolecules through refractive index sensing. Material-selective surface functionalization allows targeted immobilization of probe molecules exclusively on the waveguide sensing areas, enhancing sensitivity - down to ppt levels - and specificity. I demonstrate the successful detection of multiple biomarkers with this novel system, including DNA and polycyclic aromatic hydrocarbons, as well as selectivity of chiral enantiomers of the amino acid phenylalanine (Ligterink et al. in prep.).

Next, I will outline the future development of the LMC. By integrating light sources, detectors, and microfluidic sample handling on a single chip, the size and complexity will be reduced compared to previous systems. The compact, integrated design eliminates the need for external optical components while maintaining high sensitivity, making it particularly suitable for space applications where size, mass, and robustness are critical. This work represents a significant step toward developing field-deployable molecular detection capabilities for planetary exploration.

 

Sims et al. 2012: Sims, M.R., Cullen, D.C., Rix, C.S., Buckley, A., Derveni, M., Evans, D., García-Con, L.M., Rhodes, A., Rato, C.C., Stefinovic, M. and Sephton, M.A., 2012. Development status of the life marker chip instrument for ExoMars. Planetary and Space Science, 72(1), pp.129-137.

How to cite: Ligterink, N. F. W.: The Next-Generation Life Marker Chip: A Photonic Biosensor for Space Exploration, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4996, https://doi.org/10.5194/egusphere-egu25-4996, 2025.

EGU25-5152 | ECS | Posters on site | PS7.2

Opportunistic LEO spacecraft observation with space-borne sub-THz ISAR imaging 

Gruffudd Jones, Morgan Coe, Lily Beesley, Theo Hart, Emmanuel Karikari, Francis Pope, Marina Gashinova, and Leah-Nani Alconcel

The proliferation of space objects is increasingly becoming a large concern, with mega-constellations in low Earth orbit (LEO) exponentially increasing active spacecraft numbers, now over eleven thousand. The Pervasive Sensing group at the University of Birmingham is exploring a method of opportunistic observations of these spacecraft from a dedicated satellite equipped with a high-resolution sub-THz inverse synthetic aperture radar (ISAR) imaging payload [1]. The work includes orbit identification, optimised conjunction analysis and encounter parametrisation. We also demonstrate the use of a novel radar simulation technique – the Graphical Electromagnetic ISAR Simulator for Sub-THz waves (GEIST) [2] – to synthesise large datasets of radar images from diverse perspectives. This is linked with the Pervasive Sensing group’s development of heuristic and ML-based classification techniques [3] to identify satellite anomalous behaviour and/or damage to external infrastructure.

[1] E. Marchetti et al., "Space-Based Sub-THz ISAR for Space Situational Awareness—Concept and Design," in IEEE Transactions on Aerospace and Electronic Systems, vol. 58, no. 3, pp. 1558-1573, June 2022, doi: 10.1109/TAES.2021.3126375

[2] G. Jones et al., "Novel Simulation Method for Sub-THz ISAR Imaging of Space Objects," 2024 21st European Radar Conference (EuRAD), France, pp. 272-275, doi: 10.23919/EuRAD61604.2024.10734967.

[3] M. Coe et al., "Segmentation and Classification of Sub-THz ISAR Imagery," 2024 International Radar Symposium (IRS), Poland, pp. 233-238, ieeexplore.ieee.org/document/10645054

How to cite: Jones, G., Coe, M., Beesley, L., Hart, T., Karikari, E., Pope, F., Gashinova, M., and Alconcel, L.-N.: Opportunistic LEO spacecraft observation with space-borne sub-THz ISAR imaging, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5152, https://doi.org/10.5194/egusphere-egu25-5152, 2025.

EGU25-6435 | Posters on site | PS7.2

Solar energetic particle instrument SP@M for ESA M7 mission candidate M-MATISSE 

Lubomir Prech, Quentin Nenon, Pierre Devoto, Nicolas André, Vincent Thomas, Frantisek Nemec, and Beatriz Sanchez-Cano

M-MATISSE is one of the three mission candidates for the ESA M7 science mission call, all currently passing the Phase A with selection of the mission expected in the middle of 2026 and a possible launch at 2037. The M-MATISSE proposal involves two spacecraft (Henri and Marguerite) with almost identical scientific payload to investigate the Mars plasma environment from two vantage points on different elliptical orbits simultaneously. The main goal of M-MATISSE is, for the first time at Mars in its complexity, to explore, characterize and ultimately understand the global dynamic response of the near-Mars plasma environment to solar wind dynamics, solar energetic events and flares. In the scope of the mission is to study the dynamics induced at Mars’ environment during quiet and extreme solar wind conditions, i.e. space weather effects on the system, including the crucial lower layers of the ionosphere connecting the Mars surface and space, so far only infrequently sampled by existing missions. Also, M-MATISSE would provide essential data to enable forecasting of potential global hazard situations in robotic and human exploration of Mars. The proposed M-MATISSE configuration involves six scientific instruments on both spacecraft, two of them being actually consortia of several scientific sensors with common data processing units.

The Solar Particle at Mars (SP@M) experiment is a part of the Mars Ensemble of Particle Instruments (M-EPI) suite of three particle sensors. SP@M will study distributions of 30 keV to 1 MeV electrons and 30 keV to 10 MeV ions with 4 electron and 4 ion telescopes per spacecraft aiming to monitor parallel/antiparallel/ perpendicular to interplanetary magnetic field fluxes of energetic particles. In this contribution we focus on the description of the SP@M design as achieved in the middle of the Phase A, ongoing development activities incl. digital signal processing and electron-ion discrimination, and performance simulations. The scientific tasks of SP@M will be presented as well.

How to cite: Prech, L., Nenon, Q., Devoto, P., André, N., Thomas, V., Nemec, F., and Sanchez-Cano, B.: Solar energetic particle instrument SP@M for ESA M7 mission candidate M-MATISSE, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6435, https://doi.org/10.5194/egusphere-egu25-6435, 2025.

EGU25-6634 | Orals | PS7.2

Seismology on Venus: from measurement concepts to implementation in a planetary mission 

Raphael F. Garcia, Matthias Grott, and Iris Van Zelst and the ISSI team "Seismicity on Venus: Prediction and Detection"

The deployment of surface seismometers on the Moon and Mars has demonstrated their ability to recover both internal structure and seismicity of these planetary bodies.

However, on planets with dense atmospheres and extreme surface conditions like Venus, seismometers deployed at the surface face significant challenges, including short measurement durations due to the high temperature limitations of the electronics and elevated background noise due to ground deformations generated by atmospheric dynamics. However, the relatively unconstrained internal structure of Venus is an important missing piece in our understanding of the formation and evolution of Solar System planets.

In response, atmospheric seismology measurement concepts that rely on detecting infrasound generated by seismic waves -- already successfully demonstrated on Earth – are being explored for Venus exploration. In this context, we present a comparison of the seismic wave detection capabilities for ground based sensors, atmospheric balloon sensors, and airglow imagers measurements concepts. We then examine the scientific potential of different airglow imager configurations, demonstrating not only their relevance for Venus seismology but also their applicability to broader, high-level science questions. Furthermore, we address technical challenges associated with such a mission concept. are also discuss. These discussions provide valuable insights for the design of future missions to explore Venus’ seismicity and internal structure.

How to cite: Garcia, R. F., Grott, M., and Van Zelst, I. and the ISSI team "Seismicity on Venus: Prediction and Detection": Seismology on Venus: from measurement concepts to implementation in a planetary mission, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6634, https://doi.org/10.5194/egusphere-egu25-6634, 2025.

EGU25-7092 | Orals | PS7.2

Superresolution color images of Mars and Deimos acquired by the Hyperscout-H hyperspectral imager aboard the Hera mission 

Björn Grieger, Julia de León, Hannah Goldberg, Tomas Kohout, Gábor Kovács, Michael Küppers, Balázs Vince Nagy, Marcel Popescu, and George Prodan

The Hera mission was launched on 7 October 2024 and will reach its destination, the binary asteroids Didymos and Dimorphos, in late 2026. Hera carries the hyperspectral imager Hyperscout-H. Its sensor consists of 2048 × 1088 pixels arranged in macro pixel blocks of 5 × 5 pixels. The 25 pixels of each block are covered with filters in 25 different wavelengths where the center response ranges from 657 to 949 nm. Therefore, each of the 2048 × 1088 micro pixels provides brightness information for one wavelength, and the actual macro pixel resolution is only about 409 × 217 pixels. Any simple interpolation approach between micro pixels is strongly affected by pixel-to-pixel variations in spectra and by varying albedo and shading effects caused by surface inclination. This makes the resultant spectra very noisy.

To retrieve more accurate spectra with higher spatial resolution, we have developed a family of novel demosaicing methods. We separate the spectrum at each micro pixel into a normalized spectrum and a brightness scaling factor. Ratios of measured values from adjacent pixels are used to iteratively compute the normalized spectra, which are then brightness scaled to reproduce the measured values. This approach allows replenishment of the complete data cube of 2048 × 1088 × 25 pixels.

Four days after launch, the three cameras aboard Hera acquired images of the Moon and the Earth. Because of the large distance, the resolution of these images was limited. However, the Hyperscout-H images of the Earth demonstrated that color images at full micro pixel resolution can be reconstructed from the replenished data cube.

On 12 March 2025, Hera will perform a fly-by of Mars, and images of Mars and Deimos will be acquired from distances of about 20,000 and 1,000 km, respectively. Hyperscout-H is planned to acquire one image with both Mars and Deimos in the field of view. We will apply our demosaicing methods to replenish the complete data cubes and reconstruct color images at full micro pixel resolution.

How to cite: Grieger, B., de León, J., Goldberg, H., Kohout, T., Kovács, G., Küppers, M., Nagy, B. V., Popescu, M., and Prodan, G.: Superresolution color images of Mars and Deimos acquired by the Hyperscout-H hyperspectral imager aboard the Hera mission, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7092, https://doi.org/10.5194/egusphere-egu25-7092, 2025.

EGU25-7170 | Orals | PS7.2

The Unique Observation Geometries of Juno’s Radio Occultations of the Galilean Satellites  

Dustin Buccino, Andrea Caruso, Luis Gomez Casjus, Marzia Parisi, Marco Zannoni, Edoardo Gramigna, Drew Coffin, Paul Withers, Paolo Tortora, Ryan Park, and Paul Steffes

During Juno’s extended mission, the spacecraft performed four close flybys of the Galilean satellites. Each encounter with a Galilean satellite occurred during the ascending node crossing of the orbit and reduced the orbital period of the spacecraft, phasing the orbit for the subsequent encounter. During each encounter, a radio occultation experiment could be performed using Juno’s radio science instrumentation. During the Ganymede encounter in June 2021 and Europa encounter in September 2022, occultations of the moon’s ionospheres were performed. Both yielded detections of the moon’s ionospheres, with the Ganymede occultation revealing the importance of electron impact ionization. During the close encounters with Io in December 2023 and February 2024, although the spacecraft was not occulted by the limb of the moon, it was occulted by the Alfven wing connecting Io to Jupiter. Increased electron density was detected in the Alfven wing with the occultation method for the first time, providing independent verification of in-situ measurements of the wing. The unique observation geometries of each of these four flybys – a consequence of the complex interaction between Jupiter’s magnetosphere and the moons – required adapting traditional radio occultation techniques to invert the radio frequency measurements into electron density estimates.

How to cite: Buccino, D., Caruso, A., Gomez Casjus, L., Parisi, M., Zannoni, M., Gramigna, E., Coffin, D., Withers, P., Tortora, P., Park, R., and Steffes, P.: The Unique Observation Geometries of Juno’s Radio Occultations of the Galilean Satellites , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7170, https://doi.org/10.5194/egusphere-egu25-7170, 2025.

EGU25-8332 | Posters on site | PS7.2

HyperLab Project 

Francesco Carraro, Cristian Carli, and Sergio Fonte

In contemporary laboratory settings, there is a need for flexible and immediate approaches to updating, sharing, and analyzing acquired data. With this vision in mind, we initiated the development of the SLab Tools package at INAF-IAPS, which supports the Spectroscopy Laboratory (SLAB) dedicated to visible and near-infrared reflectance spectroscopy. SLab Tools comprises a database, a web app, and a Windows 10/11 app designed to streamline laboratory work.

As we developed the components, we decided to enhance the initial idea by transforming the SLab-dedicated app into a more general and flexible multi-platform app, offering a broader range of features. Consequently, the project was renamed HyperLab.

HyperLab aims to provide seamless access to SLab data and various statistical algorithms. It is also gaining the capability to open and analyze scientific files saved in the PDS format. Key goals of the project include: a) Simplifying routine tasks for laboratory personnel by relating multiple acquisitions and correlating them with supplementary information on measurements and samples. b) Enhancing the value of scientific data by sharing it with the research community. c) Providing the community with a modern tool that can be accessed via phone or tablet.

HyperLab's features include applying smoothing functions, calculating a continuum-removed spectrum with real-time visualization, and computing common absorption band parameters such as band center, band depth, and band area.

Significant effort has been invested in developing features related to the SLab setup, which played a crucial role at the project's inception. This includes allowing users to apply different data analysis techniques to spectra and accessing ancillary information such as sample type, category (mineral, rock, meteorite, synthetic), and acquisition geometry.

Both the web application and the multi-platform app are designed to offer the same comprehensive functionalities when working with SLab data, ensuring users can seamlessly switch between platforms without losing access to any features. The web app plays a pivotal role in the overall architecture by functioning as both the back-end for the multi-platform app and a self-contained web tool. It is responsible for managing data searches and handling the saving and retrieval of data from the database.

 

Acknowledgments:  This project was funded by INAF in 2023 under the ‘Call for Funding of Fundamental Research 2023’, in the Data Analysis Grant category.

How to cite: Carraro, F., Carli, C., and Fonte, S.: HyperLab Project, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8332, https://doi.org/10.5194/egusphere-egu25-8332, 2025.

EGU25-8702 | ECS | Posters on site | PS7.2

Influence of sensor noise levels on magnetometer calibration parameters 

Gerlinde Timmermann, Patrick Kolhey, Hans-Ulrich Auster, Ingo Richter, and Ferdinand Plaschke

Magnetometers are prime instruments of scientific spacecraft targeting the space plasma environments of solar system bodies. Despite extensive ground calibration efforts, regular inflight calibration activities of these magnetometers have shown to be crucial to maintain necessary data quality levels over time. Classically, 12 parameters influence the calibration: 3 gain values, 6 angles defining magnetic sensor orientations, and 3 zero level offsets that correspond to instrument outputs in vanishing ambient fields. Particularly in low fields, accurate choice of offset levels are of utmost importance. To achieve this, measurements of Alfvénic fluctuations in the solar wind are typically used. We investigate the influence of sensor noise levels on the accuracy of different calibration parameters, particularly on the offsets, using THEMIS/ARTEMIS magnetic field measurements. 

How to cite: Timmermann, G., Kolhey, P., Auster, H.-U., Richter, I., and Plaschke, F.: Influence of sensor noise levels on magnetometer calibration parameters, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8702, https://doi.org/10.5194/egusphere-egu25-8702, 2025.

EGU25-9964 | ECS | Orals | PS7.2

Optimising the Design of Spaceborne Time-of-Flight Mass Spectrometers with Particle Swarm Algorithms 

Robin F. Bonny, Audrey E. Aebi, Rico G. Fausch, Antea C. Doriot, Daniel R. Müller, and Martin Rubin

A time-of-flight mass spectrometer (TOF-MS) separates charged particles by their mass-per-charge ratio on the basis of their transit times through an electric field. For accurate mass determination, ions must be guided from the source inlet, through the ion-optical system, and onto the detector as a beam with a controlled, narrow opening angle. This requires careful dimensioning of the electrodes and computation of the applied electric fields to control beam deflection and achieve both spatial and temporal focusing across the entire detector plane. The primary goal of this work is to develop an efficient optimisation framework for TOF-MS ion-optical designs that addresses performance trade-offs and computational challenges. For spaceborne instrumentation, high sensitivity and resolution must be balanced against size and mass constraints, making their design and optimisation particularly challenging.

The ion-optical design process involves trading off numerous interdependent parameters without an analytical solution. Mathematically, this problem can be interpreted as a derivative-free constrained optimisation problem with high dimensionality. Bieler et al. (2011) successfully used an adaptive particle swarm algorithm (APSA) to optimise voltages and electric fields for several existing ion-optical systems [1], including the Reflectron TOF (RTOF) mass spectrometer flown on the Rosetta mission of the European Space Agency. However, their approach focused on optimising voltages for predefined ion-optical geometries, without addressing the simultaneous optimisation of geometry and voltages during the early design phase. This limitation restricts the flexibility of the optimisation process and may lead to suboptimal ion focusing.

This work fills that gap by applying a particle swarm algorithm during the early design phase of a novel TOF-MS instrument. Using the SIMION® ion and electron optics simulator [2] at its base, this approach simultaneously optimises both the electrode geometries and the applied voltages, resulting in more precise control over the electric field profiles. Additionally, parallel computation techniques are implemented at thread and process levels to efficiently manage a large number of degrees of freedom, reducing computation time by allowing multiple independent particle swarms to explore the solution space concurrently. This approach provides a scalable framework for designing more precise and computationally efficient spaceborne TOF-MS instruments, contributing to the development of next-generation instruments for planetary exploration and scientific research.

 

[1] A. Bieler, K. Altwegg, L. Hofer et al., ‘Optimization of mass spectrometers using the adaptive particle swarm algorithm,’ Journal of Mass Spectrometry, vol. 46, no. 11, pp. 1143–1151, 2011, issn: 1096-9888. doi: 10.1002/jms.2001.

[2] D. A. Dahl, ‘Simion for the personal computer in reflection,’ International Journal of Mass Spectrometry, Volume 200: The state of the field as we move into a new millenium, vol. 200, no. 1, pp. 3–25, 25th Dec. 2000, issn: 1387-3806. doi: 10.1016/S1387-3806(00)00305-5.

How to cite: Bonny, R. F., Aebi, A. E., Fausch, R. G., Doriot, A. C., Müller, D. R., and Rubin, M.: Optimising the Design of Spaceborne Time-of-Flight Mass Spectrometers with Particle Swarm Algorithms, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9964, https://doi.org/10.5194/egusphere-egu25-9964, 2025.

EGU25-10176 | ECS | Posters on site | PS7.2

COSSTA-PL - Low-pressure sensor for Dragonfly entry capsule 

Iina Jaakonaho, Maria Hieta, Maria Genzer, Jouni Polkko, Thomas Thiele, Ari-Matti Harri, and Ali Gülhan

NASA's upcoming Dragonfly rotorcraft mission is planned to be deployed to the surface of Saturn’s moon Titan [1]. As part of the Dragonfly Entry Aerosciences Measurements (DrEAM) suite [2], the Dragonfly entry capsule will include a subsystem known as the COmbined Sensor System for Titan Atmosphere (COSSTA). This subsystem is being developed by the Supersonic and Hypersonic Technologies Department at the DLR Institute of Aerodynamics and Flow Technology, in collaboration with NASA. One of the components of COSSTA is a pressure sensor developed by the Finnish Meteorological Institute (FMI). This sensor, named COSSTA-PL, is designed to measure static pressure on the entry capsule's backshell.

The sensor is based on FMI’s pressure sensors previously developed for Mars landers, mostly sharing its design with MEDA PS [3], the pressure sensor of the Perseverance rover. Its core components, the Barocap® pressure sensor heads, are developed by Vaisala. The optimal measurement range of COSSTA-PL is up to about 10 hPa, but it has a capability to measure pressures up to at least 20 hPa.

Due to possible exposure to extremely cold temperatures during the long cruise, several tests have been performed with a prototype model and individual components to confirm that the sensor endures temperatures down to -150 °C. The pressure calibration is planned to be performed mainly at FMI in the 0 to 20 hPa pressure range and -70 to +55 °C temperature range, and calibration down to -150 °C (TBC) is continued at the COSSTA level.

References

[1] Lorenz, R. D. et al. (2018). Dragonfly: A Rotorcraft Lander Concept for Scientific Exploration at Titan, Johns Hopkins APL Technical Digest 34(3), pp. 374-387.

[2] Brandis, A. et al. (2022). Summary of Dragonfly’s Aerothermal Design and DrEAM Instrumentation Suite, 9th International Workshop on Radiation of High Temperature Gases for Space Missions, 12 – 16 Sep 2022, Santa Maria, Azores, Portugal.

[3] Jaakonaho, I. et al. (2023). Pressure sensor for the Mars 2020 Perseverance rover, Planetary and Space Science 239, 105815, https://doi.org/10.1016/j.pss.2023.105815.

How to cite: Jaakonaho, I., Hieta, M., Genzer, M., Polkko, J., Thiele, T., Harri, A.-M., and Gülhan, A.: COSSTA-PL - Low-pressure sensor for Dragonfly entry capsule, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10176, https://doi.org/10.5194/egusphere-egu25-10176, 2025.

EGU25-10630 | ECS | Posters on site | PS7.2

Post Launch Performance of a Hot Cathode for Electron Ionization of a Space Borne Time-of-Flight Mass Spectrometer (NIM on board JUICE) 

Samuel Stefan Wyler, Rico Fausch, Audrey Vorburger, and Peter Wurz

On 14 April 2023, the JUICE spacecraft was launched to the Jovian system to study the emergence of potentially habitable worlds around gas giants. The Neutral-Ion Mass Spectrometer (NIM), developed by the University of Bern, will characterise the atmospheres of the Galilean moons and analyse subsurface material ejected by Europa’s plumes. NIM uses a power-efficient hot cathode filament which creates an electron beam to ionize atoms and molecules for mass spectrometric analysis.

For this mission, we employ customized yttrium oxide (Y2O3) cathodes produced by Kimball Physics, based on the ES-525 design. For example the filament legs are lengthened to minimize heat loss through conduction. Additionally, a thicker coating is applied to enhance longevity. Given the criticality of correct cathode operation, two cold-redundant cathodes are installed in the NIM instrument.

This study compares the performance of the space-qualified cathodes in the Proto Flight Model (PFM) instrument, post-launch (in orbit) commissioning, with both expected performance metrics and laboratory-tested cathodes in the Flight Spare (FS) instrument.
During commissioning, the PFM cathodes underwent conditioning lasting several hours. While both cathodes were successfully conditioned, cathode 2 exhibited performance comparable to FS cathodes, whereas cathode 1 deviated from the pre-flight performance. This deviation was further investigated through additional investigations and tests. Preliminary findings suggest that launch-induced vibrations caused slight bending of the cathode legs, resulting in asymmetry between the emitting disk and the surrounding repeller electrode.

The cathodes operate within a nominal emission range of 100 to 300 μA. Without active beam shaping, power consumption varies between 1.2 and 1.6 W (up to 1.8 W for the deviating PFM cathode 1) with a current draw of 860 to 980 mA (up to 1030 mA). Optimal beam shaping increases the current requirement by approximately 20 mA. Despite limited available data, we successfully fit our measurements to the Richardson-Dushman equation, describing the relation between operation parameters and emission current, enabling a comparison with theoretical emission expectations.

The heating current drawn by the cathode is expected to increase over the long term (up to a lifetime of 10,000 operational hours) due to degradation of the coating. In contrast, short-term behaviour (up to 100 hours) reveals a "learning" effect: cathodes exhibit improved performance when used under specific active beam-shaping configurations, an effect disrupted after exposure to air.

During the post-launch commissioning of the cathodes in orbit, the LV subsystem was commissioned as well. The commissioning, including the cathodes, bake-out heater, low-voltage electrodes, as well as the necessary electronics was successful. Long-term monitoring of the cathodes' performance in both laboratory and space environments continues.

 

How to cite: Wyler, S. S., Fausch, R., Vorburger, A., and Wurz, P.: Post Launch Performance of a Hot Cathode for Electron Ionization of a Space Borne Time-of-Flight Mass Spectrometer (NIM on board JUICE), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10630, https://doi.org/10.5194/egusphere-egu25-10630, 2025.

EGU25-10818 | Orals | PS7.2

Exploring Mars on Earth: Scientific Outcomes of the AMADEE-24 Mission   

Seda Özdemir-Fritz and Gernot Groemer

The AMADEE-24 mission, conducted by the Austrian Space Forum (ÖWF) in March and April 2024 in Armenia, was a high-fidelity Mars analog mission aimed at preparing for future human exploration of the Red Planet. The mission brought together scientists and engineers from across the globe to test innovative technologies, operational workflows, and scientific methods in a Martian-like environment. By simulating the challenges of human-robotic exploration, AMADEE-24 focused on optimizing the science return of future crewed missions to Mars and advancing planetary research.

The Armenian test site was selected for its geological and environmental similarities to Mars, offering a unique analog terrain to conduct field experiments in geology, planetary geology, astrobiology, engineering, and human factors research and testing exploration strategies and scientific instruments. It addressed key scientific and operational objectives, including the validation of exploration technologies, the refinement of mission protocols, and the development of new approaches for conducting science in remote environments.

One of the core focuses of AMADEE-24 was planetary geology and astrobiology. The analog astronauts, equipped with state-of-the-art tools such as Raman spectrometers and remote sensing devices, conducted fieldwork to investigate the mineral composition of the terrain and search for biosignatures—indicators of potential past or present life.

The mission also placed significant emphasis on human factors and mission operations. AMADEE-24 tested EVA protocols, communication strategies with Mission Support under time delay, and astronaut performance in isolation. These studies provided crucial data on the efficiency and safety of crewed operations in extreme environments, helping to optimize decision-making processes and workflows for future Mars missions.

AMADEE-24 also served as a testbed for new exploration tools. The mission tested drones, autonomous systems, and other robotic technologies in the challenging Armenian terrain. The validation of these tools in a Mars-like environment ensures that future exploration missions will be equipped with robust, reliable instruments capable of collecting high-quality scientific data under harsh conditions.

Mission requires a critical operation on payload management during AMADEE-24, which was essential for the efficient execution of the mission's science objectives. Here, we also present, the complexity of managing scientific payloads in a Mars analog environment required careful planning to ensure optimal use of instruments and seamless integration of scientific and operational workflows. The results of this operation provide insights into payload prioritization, instrument deployment strategies, and data handling processes.

The scientific outcomes of AMADEE-24 are expected to make contributions to planetary exploration research. The mission’s findings will help refine science protocols, improve instrumentation strategies, and enhance comparative planetology studies. The interdisciplinary nature of the mission, involving scientists from various fields, highlights the importance of collaboration in addressing the complex challenges of human Mars exploration.

AMADEE-24 marked a significant milestone in Mars analog research, providing valuable insights into the science, technology, and human factors that will shape future crewed missions to Mars. By bridging the gap between Earth-based experiments and space missions, AMADEE-24 plays a crucial role in humanity’s preparation for the first steps on athe Martian surface.

How to cite: Özdemir-Fritz, S. and Groemer, G.: Exploring Mars on Earth: Scientific Outcomes of the AMADEE-24 Mission  , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10818, https://doi.org/10.5194/egusphere-egu25-10818, 2025.

EGU25-11879 | ECS | Orals | PS7.2

The M-MATISSE Crosslink Occultation Instrument MaCro 

Tobias Vorderobermeier, Tom Andert, Martin Paetzold, Silvia Tellman, Dirk Plettemeier, Jan Budroweit, Takeshi Imamura, Hiroki Ando, Antonio Genova, Matthias Hahn, Katsuyuki Noguchi, Janusz Oschlisniok, Kerstin Peter, Wolfgang Schäfer, Beatriz Sanchez-Cano, and Francois Leblanc

The M-MATISSE mission, currently in its Phase A study by the European Space Agency (ESA), is a Medium-class (M7) candidate that aims to explore the complex interactions between Mars' magnetosphere, ionosphere, and thermosphere (MIT coupling). This two-spacecraft mission, comprising identical payloads on board "Henry" and "Marguerite", will investigate how these interactions are influenced by space weather and the lower atmosphere. The spacecraft will follow different orbits with apocenters at 3,000 km and 10,000 km altitude, respectively, and pericenters at 250 km altitude, allowing for a comprehensive understanding of the Martian environment.

The MaCro instrument, which utilizes an inter-satellite radio link, will study occultation events in the Martian atmosphere, covering altitudes from 1,000 km to the surface, including the ionosphere and neutral atmosphere. Occultations occur when one spacecraft disappears behind the Martian disk as seen from the other spacecraft. Operating at two frequencies simultaneously—UHF and S-band—MaCro allows for a clear distinction between the ionospheric plasma and the neutral part of the atmosphere. The instrumentation setup consists of two software-defined transceivers (SDR) at UHF and S-band, stabilized by a highly stable oven-controlled crystal oscillator (OCXO) on each spacecraft. The observables include the shift of the carrier frequencies caused by the bending of the radio ray path in the atmosphere/ionosphere and the received signal power.

This presentation provides an overview of the MaCro instrument's technical concept and scientific objectives.

How to cite: Vorderobermeier, T., Andert, T., Paetzold, M., Tellman, S., Plettemeier, D., Budroweit, J., Imamura, T., Ando, H., Genova, A., Hahn, M., Noguchi, K., Oschlisniok, J., Peter, K., Schäfer, W., Sanchez-Cano, B., and Leblanc, F.: The M-MATISSE Crosslink Occultation Instrument MaCro, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11879, https://doi.org/10.5194/egusphere-egu25-11879, 2025.

EGU25-11994 | ECS | Posters on site | PS7.2

Composition Analysis of an Allende Chondrule using a Space-Prototype Laser Ablation Ionization Mass Spectrometer 

Salome Gruchola, Peter Keresztes Schmidt, Andreas Riedo, Marek Tulej, and Peter Wurz

The Allende meteorite, which fell in northern Mexico in 1969, is one of the most significant meteorites ever studied. As a carbonaceous chondrite, it represents some of the oldest and most primitive material in the solar system, dating back over 4.5 billion years. It provides insights into the early solar nebula and the processes of planetary formation. Through chemical composition analysis of the meteorite’s refractory inclusions, a deeper understanding of the building blocks of planets and the chemical evolution of our solar system can be gained [1].

In this contribution, we present the chemical composition analysis of a chondrule from the Allende meteorite. A space-prototype Laser Ablation Ionization Mass Spectrometer (LIMS) [2] was used to map a selected chondrule, and the element abundance of more than 19 elements was retrieved and quantitatively studied. The chondrule itself was identified as a porphyritic olivine, depleted in volatiles compared to the surrounding matrix. SEM-EDX and Raman spectroscopy were used for cross-validation.

Unsupervised machine learning (ML) was used to dimensionality reduce and cluster the pre-processed LIMS data to find distinct groups of different chemical compositions. This allowed the separation of the compositionally different materials present in the studied sample and allowed for their comparison [3]. The retrieved element maps suggest the presence of two rims around the chondrule, and their possible formation times and processes will be discussed in this contribution. Furthermore, another approach to reduce the dimensionality of the acquired LIMS data based on image segmentation will be presented, together with a discussion of the benefits and feasibility of applying unsupervised ML on board a spacecraft.

 

[1] Neuland, M. B. et al., 2021, doi:10.1016/j.pss.2021.105251.
[2] Riedo, A. et al., 2012, doi:10.1002/jms.3104.
[3] Gruchola, S. et al., 2024, doi:10.3847/PSJ/ad90b6.

How to cite: Gruchola, S., Keresztes Schmidt, P., Riedo, A., Tulej, M., and Wurz, P.: Composition Analysis of an Allende Chondrule using a Space-Prototype Laser Ablation Ionization Mass Spectrometer, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11994, https://doi.org/10.5194/egusphere-egu25-11994, 2025.

EGU25-12150 | ECS | Posters on site | PS7.2

Refining Non-Conservative Force Modeling of LRO for Long-Term Lunar Gravity Signals 

Ariele Zurria, Gael Cascioli, Erwan Mazarico, and Luciano Iess

Since 2009, the Lunar Reconnaissance Orbiter (LRO) has been mapping the Moon to unprecedented detail, capturing, among others, high-resolution images and altimetric profiles to acquire invaluable datasets for understanding its evolution. Transforming this wealth of data into detailed maps and terrain models depends on the accurate determination of the spacecraft's trajectory. This is achieved through a precise orbit determination process, which relies on radio tracking data acquired by ground stations. Furthermore, the orbit determination of LRO can allow scientists to refine estimates of the Moon's geophysical parameters (e.g., gravity field, tidal response), advancing our understanding of its internal structure and history (Goosens et al., 2024; Mazarico et al.,2014).

The reliability of these estimates is intrinsically tied to the accuracy of the spacecraft's orbit reconstruction. LRO's motion is influenced by various perturbative forces, among which non-conservative forces, such as the pressure exerted by solar or planetary radiation, pose significant challenges. These forces, typically small in magnitude, are complex to model accurately. An incorrect modeling of non-gravitational effects can introduce errors in orbit determination that build up over time, leading to biases in scientific measurements and potentially resulting in incorrect interpretations of the Moon's geophysical properties.

To mitigate the errors introduced by mismodelling, a multi-arc approach is typically employed in the orbit determination process, dividing the mission timeline into shorter arcs. However, this approach reduces sensitivity to long-term gravitational signals, such as those originating from the Moon’s inner core. By refining the spacecraft's dynamical model, it becomes possible to extend the duration of the arcs, potentially enabling the recovery of previously undetected signals and a better understanding of the Moon’s interior. The availability of LRO’s extensive radiometric data, recorded during intervals unaffected by wheel off-loading maneuvers, offers an ideal dataset for developing and testing more refined physical-numerical models.

This work focuses on enhancing the modeling of non-gravitational accelerations acting on the LRO to detect long-term lunar gravity signals. To address this task, we test innovative modelling techniques based on ray-tracing methods and compare them against traditional approaches to evaluate their accuracy and effectiveness. Our results show that the ray-tracing is a powerful tool to refine the dynamical model of the spacecraft for planetary geodesy and geophysics investigations. This framework not only helps obtaining an accurate trajectory reconstruction but also provides a means for gaining deeper insights into the Moon's internal dynamics, contributing to a more comprehensive understanding of its geophysical and evolutionary processes.

How to cite: Zurria, A., Cascioli, G., Mazarico, E., and Iess, L.: Refining Non-Conservative Force Modeling of LRO for Long-Term Lunar Gravity Signals, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12150, https://doi.org/10.5194/egusphere-egu25-12150, 2025.

EGU25-12796 | ECS | Posters on site | PS7.2

Survey of the estimated mass of ablated material and intact debris from 'end-of-life' LEO spacecraft entering the atmosphere 

Lily Beesley, Phineas Whitlock, Theo Hart, Emmanuel Karikari, Francis Pope, and Leah Nani-Alconcel

De-orbiting via re-entry into the Earth's atmosphere is the modus operandi of end-of-life LEO satellite disposal despite the uncertainties regarding the impact of ablated materials and intact debris. Elements that have never existed naturally within our atmosphere, such as hafnium and niobium, which originate solely from ablated satellites and rocket bodies, have already been detected in the stratosphere. This ablated material will only increase as early- and next-generation LEO constellations reach the disposal phase of their lifecycle. Starlink alone has requested to add a further 30,000 satellites to their existing mega-constellation, with others following suit. Of particular interest are the re-entry mass and fluxes of very high melting point de-orbiting materials that are unlikely to ablate, such as the laser medium used in inter-satellite optical communication links. We present the results of a preliminary study into the projected mass and geographic fluxes of ablated material and intact objects into the upper atmosphere. 

How to cite: Beesley, L., Whitlock, P., Hart, T., Karikari, E., Pope, F., and Nani-Alconcel, L.: Survey of the estimated mass of ablated material and intact debris from 'end-of-life' LEO spacecraft entering the atmosphere, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12796, https://doi.org/10.5194/egusphere-egu25-12796, 2025.

The Panel on EXploration of the Committee on SPAce Research (COSPAR) of the International Science Council (ISC) is actively preparing for the 2026 Assembly in Florence a new edition of its RoadMap for Exploration, with contributions from all relevant Scientific Commissions of COSPAR. The main goal of this RoadMap is to provide a 20-year perspective on the upcoming developments of Human and robotic exploration of the Solar System, to identify with the relevant scientific communities the greatest scientific benefits that are expected from planetary exploration, and to suggest ways to secure the largest possible scientific return from investments in exploration made by an increasingly broad spectrum of players. To achieve this goal, PEX and COSPAR will identify and promote the most promising mechanisms for international cooperation. We will identify the best practices to preserve the natural environments and sometimes sparse resources available at the different destinations in the Solar System, particularly at the Moon and Mars. We will also identify the critical technology developments needed for science, in the spirit of the Horizon 2061 foresight exercise. We will explore the best approaches for securing a sustainable exploration program offering participation opportunities to all public and private stakeholders. We will also explore the conditions that will favor an open cooperation between all these stakeholders for the benefit of scientific discoveries and of a peaceful expansion of Humankind into outer space.

In the context of the EGU, we will emphasize the outstanding contributions to this RoadMap that are expected from the European community, and engage with the audience and with EGU participants  on their participation in this new version of the COSPAR RoadMap for Exploration. 

How to cite: Blanc, M., Galli, A., and Smith, H. D.: Towards a sustainable and environment-friendly development of international cooperation in planetary exploration: building a new COSPAR Exploration RoadMap, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13179, https://doi.org/10.5194/egusphere-egu25-13179, 2025.

EGU25-13826 | Posters on site | PS7.2

2-um Differential Absorption Lidar for Martian Atmospheric CO2 and atmospheric Pressure measurements 

Joel Campbell, Zhaoyan Liu, Jihong Geng, Bing Lin, and Jirong Yu

Martian atmosphere consists dominantly of CO2 gas. Observations of atmospheric CO2 amount would provide crucial knowledge on Martian CO2 annual cycles, surface air pressure variations, and atmospheric dynamics including dust storms. This team explores a great potential to use a Martian differential absorption lidar (DIAL) operating at the 2-um CO2 absorption band for the purpose. For the considered system, closely-spaced wavelengths are selected so that Martian environmental impacts such as surface reflection, atmospheric scattering, and absorption from other trace gases on the lidar return signals are very similar, but the difference in CO2 absorption is substantial. The Martian CO2 amount and surface air pressure could be retrieved from the measured CO2 differential absorption optical depth at the selected wavelengths. Simulation studies found that return signals from the surface for a Martian space-borne CO2 DIAL system could have sufficient signal strengths that allow column CO2 amount and surface air pressure measurements with 1% and 1 Pa precision, respectively, after horizontally 5 km averaging under normal weather/dust conditions. These CO2 and pressure measurements would significantly improve Martian weather and climate modeling and prediction. Current study of the Martian CO2 DIAL system and laboratory experiments show that a 2-um CO2 DIAL system for Martian atmospheric applications can be developed with existing fiber laser and lidar technologies. These results indicate that Martian space-borne CO2 DIAL systems significantly improve next-generation Mars’ weather and climate predictions and greatly benefit future human Mars explorations. We report the latest progress in the lidar development including certain instrumentation and laboratory experimental results.

How to cite: Campbell, J., Liu, Z., Geng, J., Lin, B., and Yu, J.: 2-um Differential Absorption Lidar for Martian Atmospheric CO2 and atmospheric Pressure measurements, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13826, https://doi.org/10.5194/egusphere-egu25-13826, 2025.

EGU25-13874 | Orals | PS7.2

Gravity Science Goals for the UAE EMA Mission 

Daniel Scheeres, Jay McMahon, Jacopo Villa, Mattia Pugliatti, Margaret Landis, Paul Hayne, and Hoor AlMazmi

The UAE’s Emirates Mission to the Asteroid Belt (EMA) is scheduled to launch later this decade. The mission will rendezvous with the water-rich asteroid (269) Justitia, and along the way will flyby 6 different main belt asteroids. The EMA mission goals combine both scientific investigation on the nature of water-rich asteroids and determining the resource potential present in asteroidal bodies. While all of the asteroid flybys will be too fast to enable precise mass estimates, the rendezvous with Justitia will include estimating its mass, gravity field and internal density distribution as a main scientific goal. The approach to be taken will mimic other asteroid rendezvous missions such as NASA’s NEAR, Dawn and OSIRIS-REx missions. Specifically, a combination of optical navigation images along with radio metric tracking from the Earth during an orbital phase will be combined to determine the asteroid precise spin state, total mass, and gravity field coefficients.

 

Upon arrival at Justitia, the EMA spacecraft will first have a few flybys of the asteroid to determine its overall mass. Following this will be an extended mission phase where it will orbit the asteroid to measure its higher gravity coefficients. After the gravity field is appropriately mapped, the mission will focus on observations of its surface with multi-spectral instrumentation. While the first orbital phase is driven by navigation needs, gravity science will process tracking and optical navigation measurements through all of the orbital phases of the mission in order to produce the highest fidelity gravity field feasible.

 

This talk will introduce the specific challenges that the EMA mission will need to overcome at Justitia. Challenges and opportunities exist for the orbital phase of the mission, as depending on the precise spin state and total mass of the body, a sun synchronous orbit may be feasible and advantageous for the other imaging instruments. A key scientific result will be the bulk density measurement and comparison of the measured gravity field with the overall shape model of the asteroid, enabling constraints on the internal distribution of material in this body. The talk will also review the expected performance based on mission design and current knowledge of Justitia’s likely shape, spin and density range.

 

Funding support for the EMA project was provided by the United Arab Emirates Space Agency and its knowledge partner, the University of Colorado Boulder’s Laboratory for Atmospheric and Space Physics.

How to cite: Scheeres, D., McMahon, J., Villa, J., Pugliatti, M., Landis, M., Hayne, P., and AlMazmi, H.: Gravity Science Goals for the UAE EMA Mission, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13874, https://doi.org/10.5194/egusphere-egu25-13874, 2025.

Laboratory experiments constructed following the principle of hydrodynamic similarity often prove to be surprisingly accurate models of large-scale atmospheric flow phenomena. In the von Kármán Laboratory of Environmental Flows we designed new innovative experiment configurations, which are modified versions of the water-filled differentially heated rotating annulus setting, a widely used laboratory-scale minimal model of the mid-latitude Terrestrial atmospheric circulation. In the framework of our ESA-sponsored VERATAC (Venus Radar Topography and Atmospheric Circulation) project and in preparation for ESA's EnVision mission to Venus, we intend to model the hydrodynamic instabilities emerging in the superrotating upper atmosphere of the planet Venus, where the cloud tops circle the planet ca. 60 times faster than the rotation period of the surface. In our preliminary experiments and numerical simulations, we have explored the character of the atmospheric flow patterns developing at different values of the radial temperature gradient and rotation rate, while also applying an azimuthally (zonally) inhomogeneous, dipole-like heating and cooling along the rim of the cylindrical tank. These boundary conditions imitate the thermal driving provided by the meridional temperature contrast – yielding an Eady cell-like overturning convection on Venus – and the thermal difference between the day side and night side, both of which are essential conditions for superrotation to occur. Besides the better understanding of the Venusian atmosphere, this experimental configuration may also be a useful model of the large-scale atmospheric circulation of tidally locked exoplanets, on which a large pool of new empirical data is expected to become available in the coming decade from new space observatories.

How to cite: Vincze, M.: Laboratory-scale experimental modeling of superrotating planetary atmospheres  , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14290, https://doi.org/10.5194/egusphere-egu25-14290, 2025.

EGU25-14687 | Orals | PS7.2

Radio Occultation Observations of the Lunar Ionosphere Variations Over GRAIL Mission Period 

Yu-Ming Yang, Kamal Oudrhiri, Paul Withers, Timothy Stubbs, Daniel Erwin, and Dustin Buccino

The Signal of Opportunity using NASA’s Gravity Recovery and Interior Laboratory (GRAIL) radio signals to remotely sense the Lunar ionosphere has been successfully demonstrated. The GRAIL mission consisted of an identical pair of spacecraft approximately 100 km apart in a circular polar orbit around the Moon; during the science mission period, the GRAIL’s X-band Radio Science beacon (RSB) data provide applicability for the radio occultation of the lunar electron density profiles with the uncertainty of frequency residual measurement ~ 1 mHz corresponding to ~ 2 x 108 m-3 electron density uncertainties. We will present our observation updates of the Lunar ionosphere in terms of the near-surface electron profiles versus altitude retrieved from the RSB data to understand its spatial and temporal variations during the GRAIL science mission period. The nature of the lunar ionosphere is a long-standing mystery; GRAIL’s observations of the near-surface electron density profiles and its responses to solar winds and storms impact the near-surface plasma environment.

How to cite: Yang, Y.-M., Oudrhiri, K., Withers, P., Stubbs, T., Erwin, D., and Buccino, D.: Radio Occultation Observations of the Lunar Ionosphere Variations Over GRAIL Mission Period, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14687, https://doi.org/10.5194/egusphere-egu25-14687, 2025.

EGU25-14771 | Posters on site | PS7.2 | Highlight

Instruments  Development and Analogue Simulations: ILEWG LUNEX EMMESI EuroMoonMars Earth Space Innovation  2023-24  Highlights 

Bernard Foing and the TEAM ILEWG LUNEX EMMESI EUROMOONMARS EARTH SPACE INNOVATION 2023-24

We describe research and instruments development highlights from ILEWG LUNEX EuroMoonMars Earth Space Innovation EMMESI academy, EuroSpaceHub/GreenSpaceHub partners contributing to MoonMars and space missions, Field Research, Astronautics and Entrepreneurship. 
Sample analysis: we analysed various samples including meteorites from Moon, Mars, asteroids, and analogue field samples from campaigns (Vulcano, Etna, Hawaii HI-SEAS) using spectrometry, hyperspectral imaging and Ra-man . 
LUNEX also participates in collaboration with TU Delft in the study of ice, minerals and organics mixture relevant for Moon, Mars and icy Moons.

Payload development: we have developed a test bench for sample analysis using reflectance and transmission spec-troscopy, Raman spectroscopy and microscopy. We also adapted an Hyperspectral camera for sample analysis and for telescopic observations of the Moon and other celestial objects. Space Photonics Lab : this is being developed with in collaboration with Fotonika Latvia, with cubesat synergy  . 

Shoebox instruments for laboratory tests and analogue were developed for future Moon and Mars  missions. We are conceiving a concept of a shoebox module for extract-ing organics from icy moons of Jupiter and Saturn, with special prototype for Enceladus plumes or surface. LUNEX ExoGeoLab lander is currently adapted with  shoebox instruments for supporting future missions to Moon, Mars and icy moons. 

Cubesats for education, EarthMoonMars exploration: LUNEX EMMESI has initiated the development of univer-sity education cubesats with the support of Leiden Univer-sity (Observatory, LIACS computer science, Physics and Optics), Leiden Instrument Schools LiS, Deft TU, InHol-land Delft, ESA BIC. 

How to cite: Foing, B. and the TEAM ILEWG LUNEX EMMESI EUROMOONMARS EARTH SPACE INNOVATION 2023-24: Instruments  Development and Analogue Simulations: ILEWG LUNEX EMMESI EuroMoonMars Earth Space Innovation  2023-24  Highlights, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14771, https://doi.org/10.5194/egusphere-egu25-14771, 2025.

EGU25-14802 | Orals | PS7.2

The Lunar Dust Experiment (LDEX) as a CubeSat payload on polar orbit around the Moon  

Mihaly Horanyi and Scott Knapmiller

The Lunar Dust Experiment (LDEX) onboard the Lunar Atmosphere and Dust Environment Explorer (LADEE) mission orbited near the lunar equator for about 6 months (9/2013 - 4/2014) and discovered a permanently present dust exosphere engulfing the Moon, comprised of particles ejected from the surface by the continual micrometeoroid bombardment.  Re-flying LDEX on a polar orbit enables mapping the dust ejecta production over the entire lunar surface and improves our understanding of volatile retaining in permanently shadowed regions (PSR) and their potential for in-situ resource utilization (ISRU). The CU/LASP internally funded project is for developing a flight concept to adopt our existing LDEX Engineering Model (EM) to be accommodated onboard a CubeSat for a future flight opportunity. The LDEX EM is a fully functional instrument with a high technical readiness level (TRL 9). This CubeSat precursor will justify flying a follow-up larger mission with a more advanced dust instrument capable of in situ compositional and isotopic analysis based on impact ionization time-of-flight mass spectrometry. LASP instruments, like the Surface Dust Analyzer (SUDA) onboard the Europa Clipper mission launched in 2024, and the Interstellar Dust Experiment (IDEX) onboard the Interstellar Mapping and Acceleration Probe (IMAP) to be launched in 2025, could be used for an on-orbit exploration of the volatile content of PSRs.  This talk will summarize the LADEE/LDEX findings and the new CubeSat project, including the anticipated results from the proposed CubeSat polar mission. 



How to cite: Horanyi, M. and Knapmiller, S.: The Lunar Dust Experiment (LDEX) as a CubeSat payload on polar orbit around the Moon , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14802, https://doi.org/10.5194/egusphere-egu25-14802, 2025.

EGU25-15048 | Orals | PS7.2

Plasma Brake for Space Debris Mitigation 

Petri Toivanen, Pekka Janhunen, Jarmo Kivekäs, Jouni Polkko, Maria Genzer, Maria Hieta, and Harri Haukka

The concept of Plasma Brake is based on the ionospheric plasma Coulomb drag. It is analogous to the air drag in the neutral atmosphere. The dragging obstacle against the orbital plasma RAM flow is established by an electrostatic field with a high voltage difference with respect to the ambient plasma, typically -1 kV. The potential structure is supported by a long 4-wire tether with single aluminium wires with thickness of less than 50 um. The redundant structure makes the tether resilient against micro-meteoroids. The tether deployed by the Plasma Brake is stabilised by the gravity gradient. As the negative tether is attracting plasma ions, a current system between the tether and the ambient plasma is set up. However, the required high voltage power system and its power consumption is such that the Plasma Brake can be considered as a passive debris removal system. In addition, the hair-thin tether sets no harm to other space assets based on micro-meteoroid and space debris flux models such as MASTER-2009. In this presentation, we overview the Plasma Brake plasma physics, deorbiting capabilities, past and future CubeSat in-orbit experiments, and technology development in ESA framework.

How to cite: Toivanen, P., Janhunen, P., Kivekäs, J., Polkko, J., Genzer, M., Hieta, M., and Haukka, H.: Plasma Brake for Space Debris Mitigation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15048, https://doi.org/10.5194/egusphere-egu25-15048, 2025.

EGU25-15221 | Orals | PS7.2

IRF SpaceLab – a Swedish opening research infrastructure to support space and planetary exploration 

Mate Kerenyi, Stas Barabash, and Philipp Wittmann

Building on more than 60 years of success in experimental space research, the Swedish Institute of Space Physics (IRF) has developed a comprehensive test, qualification, and calibration infrastructure known as IRF SpaceLab. This facility supports space hardware development and manufacturing. IRF SpaceLab includes the following capabilities:

  • Co-60 Irradiation Facility: Provides dose rates ranging from 1 kR over 3.5 days to 1 kR in 5 hours, depending on the distance to the source. These moderate dose rates make the facility ideal for realistic radiation testing of space hardware.
  • Radioactive Isotope Collection: Features a wide array of isotopes for detector characterization, including Co-60, Cs-137, Ni-63, H-3, Ba-133, and Ra-226.
  • Thermal-Vacuum Chambers: Offers three chambers designed for testing hardware at different scales: board level, instrument level (<50 cm), and nano/micro-satellite scale (<1 m). The latter chamber is equipped with an LN2-cooled shroud and solar flux simulators, suitable for thermal balance tests.
  • Shaker (35 kN): Capable of mechanical testing of objects up to 100 kg in a clean environment.
  • Ion (+/-), Neutral, and Electron Beam Facility: Operates within an energy range of 50 eV to 50 keV and includes a 4-degree-of-freedom turntable.
  • Particle-Surface Interaction Facility: Designed for surface characterization, particularly for surface-based ion mass analyzers.

One of the key advantages of the IRF SpaceLab is the integration of these diverse facilities within a single premises operated under a small research institute environment. This setup minimizes formalities and administrative overhead. IRF SpaceLab is open to external users to support space and planetary exploration initiatives (https://spacelab.irf.se/).

How to cite: Kerenyi, M., Barabash, S., and Wittmann, P.: IRF SpaceLab – a Swedish opening research infrastructure to support space and planetary exploration, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15221, https://doi.org/10.5194/egusphere-egu25-15221, 2025.

EGU25-15928 | Posters on site | PS7.2

Data in the ESA Planetary Science Archive: A cookbook to access them  

Thomas Cornet, Mark S. Bentley, Daniela Coia, Ruben Docasal, Emmanuel Grotheer, David Heather, Tanya Lim, Joana S. Oliveira, Jose Osinde, Francisco Raga, Gemma Ramos, and Jaime Sainz

The ESA Planetary Science Archive (PSA) hosted at the European Space Astronomy Centre (ESA/ESAC) is a multi-mission archive currently supporting ten planetary missions, from missions beyond their post-operations phase to missions currently being operated. The data are being archived following the NASA Planetary Data System (PDS) Standard (version 3 or 4, depending on the mission). Missions currently in operations or within their cruise phase, such as ExoMars Trace Gas Orbiter (TGO), BepiColombo, and JUICE, archive the data in PDS4 format and follow the concept of operational archiving, where data are regularly generated and delivered to the PSA in small batches (e.g. daily). The PSA provides various means to access these data: through a web User Interface (UI), a secure FTP server, or via programmatic access with the EuroPlaNet Table Access Protocol (EPN-TAP) to the data holdings. The PSA supports data access with different proprietary status (either public or private when within their proprietary period) to ensure adequate support to the mission instrument teams. Ongoing developments with the integration of the PSA in the ESA Datalabs platform open additional ways to access and visualise the data directly from a web browser. In this work, we will illustrate the different means of searching for, downloading, and using the PDS4 planetary data archived in the PSA. 

How to cite: Cornet, T., Bentley, M. S., Coia, D., Docasal, R., Grotheer, E., Heather, D., Lim, T., Oliveira, J. S., Osinde, J., Raga, F., Ramos, G., and Sainz, J.: Data in the ESA Planetary Science Archive: A cookbook to access them , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15928, https://doi.org/10.5194/egusphere-egu25-15928, 2025.

EGU25-16350 | Orals | PS7.2

Venus' rotation state using Venus Express tracking data and expected outcomes for the EnVision radio-science experiment. 

Maëva Lévesque, Pascal Rosenblatt, Jean-Charles Marty, and Caroline Dumoulin

The main characteristic of Venus that distinguishes it from the other planets is its rotation period, which is very long at 243 Earth days. Although several solutions of this period have been determined using different methods (either from Venus’s orbit or from Earth), this parameter remains poorly constrained. In particular, there is a difference of 7 minutes between the lowest and highest estimates of the rotation period. Currently, only a 3 minute variation in the Length Of the Day (LOD) can be explained by modeling various effects such as the tidal torque exerted on Venus by the Sun and the coupling between the atmosphere and the planet. In our study, we propose a new estimate of the rotation period of Venus using Doppler tracking data from the Venus Express spacecraft. The Venus Express (VEX) mission was launched by the European Space Agency (ESA) in November 2005 and orbited Venus for almost 8 years. The main objective of the mission was to study the planet's atmosphere. To determine a new solution for the rotation period of Venus, we use the Precise Orbit Determination (POD) method, which involves a least-squares adjustment of the difference between the Doppler data collected on Earth and the Doppler data obtained by the numerical integration of forces that can affect the spacecraft's motion. We found a rotation period for Venus of 243.0200 ± 0.0007 days, within the range of values reported in the literature and obtained using different methods and databases. However, the expected periodic variations in the rotation period or the precession rate could not be detected due to the lack of sensitivity of Doppler measurements in the signature of these parameters on the VEX’s trajectory. ESA's EnVision mission, scheduled for launch around 2031, aims to study Venus from its deep core to the top of its atmosphere. We have carried out simulations to predict EnVision's performance. The predicted uncertainty in the rotation period is 0.6 seconds, compared to the uncertainty of 1 minute obtained with VEX. For the precession rate, the predicted uncertainty is 0.2%, compared to 7% obtained with ground-based radar data. The near-polar and low eccentricity of the spacecraft's orbit will provide greater sensitivity to the planet's rotational state.

How to cite: Lévesque, M., Rosenblatt, P., Marty, J.-C., and Dumoulin, C.: Venus' rotation state using Venus Express tracking data and expected outcomes for the EnVision radio-science experiment., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16350, https://doi.org/10.5194/egusphere-egu25-16350, 2025.

EGU25-16492 | ECS | Posters on site | PS7.2

Estimation of Spacecraft Outgassing During the Lunar-Earth Gravity Assist of JUICE Using Radiometric Observations  

Paolo Cappuccio, Andrea Sesta, Thomas Syndercombe, Umberto De Filippis, Daniele Durante, Mauro Di Benedetto, and Luciano Iess

The JUpiter ICy moons Explorer (JUICE), the European Space Agency’s first large-class mission under the Cosmic Vision 2015–2025 program, is dedicated to exploring the potential habitability of Jupiter’s icy moons: Europa, Callisto, and Ganymede. Launched on April 14, 2023, JUICE is currently in an 8-year cruise phase to Jupiter, utilizing gravity assists from Venus, Earth, and the Moon. Notably, JUICE is the first spacecraft to execute a Lunar-Earth gravity assist (LEGA), which was successfully completed in August 2024. This maneuver provided a critical trajectory adjustment while also allowing several onboard instruments to operate during the flyby.

Shortly after the Moon gravity assist, JUICE experienced an unforeseen acceleration attributed to an outgassing event. During the LEGA, radiometric observables, including Doppler and ranging data in the X-band, were collected by ESA’s New Norcia deep space station. These measurements were analyzed to characterize the outgassing-induced delta-V acting on JUICE. The analysis involved reconstructing the outgassing event and comparing it with models. The characterization of this event using radiometric data provides insights that complement measurements from other onboard instruments. For instance, the spacecraft’s reaction wheels recorded an excess torque as they compensated for the perturbation to maintain attitude control. The High-Accuracy Accelerometer (HAA), the Particle Environment Package (PEP), and the Submillimetre Wave Instrument (SWI) also captured data related to the outgassing event, enhancing its overall characterization.

In this work, we analyze radiometric measurements to provide a detailed quantification of the magnitude and orientation of the outgassing force during the flyby. These findings improve our understanding of non-gravitational forces affecting JUICE and contribute to refining our knowledge of the spacecraft's dynamical environment.

How to cite: Cappuccio, P., Sesta, A., Syndercombe, T., De Filippis, U., Durante, D., Di Benedetto, M., and Iess, L.: Estimation of Spacecraft Outgassing During the Lunar-Earth Gravity Assist of JUICE Using Radiometric Observations , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16492, https://doi.org/10.5194/egusphere-egu25-16492, 2025.

EGU25-16587 | ECS | Orals | PS7.2

Two years of observations with the JUICE mission radiation monitor, RADEM. 

Marco Pinto, Laura Rodríguez-García, Francisca Santos, Nina Dresing, Rami Vainio, Christina Cohen, Erika Palmerio, Patrícia Gonçalves, Nicolas Altobelli, Olivier Witasse, Giovanni Santin, Ry Evill, and Arlindo Marques

Jupiter and its icy moons—Europa, Ganymede, and Callisto—are among the most intriguing targets in the Solar System for studying habitability and searching for life. Substantial evidence suggests that these moons harbor subsurface water oceans beneath their icy crusts, with conditions that may support the development and sustainability of life. To investigate this, the European Space Agency (ESA) has launched the JUpiter ICy moons Explorer (JUICE) on April 14th, 2023.

The Jovian radiation environment is extremely hazardous for space exploration. High-energy electrons trapped in the Jovian system can penetrate thick shielding walls and accumulate large doses in electronic components and materials reducing their operational lifespan significantly. High energy particles can also disassociate biological molecules that migrated from the icy moons’ oceans to the surface hindering the detection of biosignatures from orbit.

For these reasons, JUICE carries a RADiation hard Electron Monitor (RADEM), with a novel design, capable of measuring high energy electrons, protons, and ions. RADEM is an engineering instrument, that is continuously operated throughout the mission including its cruise phase, but that can also contribute significantly to scientific investigations of the Jovian system. The same is true for the cruise phase. JUICE joins an increasing but still limited Solar fleet that includes STEREO-A, Solar Orbiter, Parker Solar Probe, BepiColombo, and near-Earth spacecraft, having already observed dozens of Solar Energetic Particle events.

In this work, we will take a deep dive into the two first years of RADEM observations, calibration activities, and scientific highlights, including a cosmic ray calibration campaign, cross-calibrations with STEREO-A and SOHO, and observation of the Van Allen belts during JUICE’s world first Lunar-Earth Gravity Assist.

How to cite: Pinto, M., Rodríguez-García, L., Santos, F., Dresing, N., Vainio, R., Cohen, C., Palmerio, E., Gonçalves, P., Altobelli, N., Witasse, O., Santin, G., Evill, R., and Marques, A.: Two years of observations with the JUICE mission radiation monitor, RADEM., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16587, https://doi.org/10.5194/egusphere-egu25-16587, 2025.

EGU25-16961 | ECS | Orals | PS7.2

Geodetic Modeling of Gas Giants: An Integrated Approach Applied to Jupiter 

Matteo Fonsetti, Andrea Caruso, Marco Zannoni, Paolo Tortora, Eli Galanti, Yohai Kaspi, and Maria Smirnova

Geodetic calculations concerning gaseous giants hold great importance in planetary astrophysics and fundamental physics, as they provide critical insights into planetary structure, dynamics, and evolution. Advancing our understanding of the shape of gaseous planets is essential for improving the precision of radio occultations—a remote sensing technique used to sound the atmospheres of celestial bodies. Accurate shape modeling also contributes to better constraining interior models, allowing for a deeper understanding of the physical processes governing gas giants and other celestial bodies, including Earth. Such advancements are not only key for refining our knowledge of planetary dynamics but also offer valuable insights into the formation of our stellar system and similar planetary systems. Additionally, these developments facilitate the characterization of exoplanetary atmospheres, which is vital for the study of planets beyond.

The shape of a fluid, rotating celestial body is primarily determined by its rotation rate and internal density distribution, which together define the planet's gravitational potential. This shape is further refined by the effects of zonal winds, which introduce an additional centrifugal term, generating perturbations that can significantly deviate from the profile expected for a solid rotating body. These perturbations are particularly pronounced at low latitudes, where the centrifugal component is most significant. We present a method, building on the approaches of Lindal et al. (The Astronomical Journal, Vol. 90, n. 6, 1985) and Galanti et al. (GRL, Vol. 50, e2022GL102321, 2023), to calculate the shape of a gas giant by harmoniously integrating data from gravity experiments, wind measurements, and radio occultation observations. This integrated methodology allows for a precise estimation of the planet's shape, accounting for both its internal structure and atmospheric dynamics. The results obtained from applying this method to a real case will be illustrated, with a focus on Jupiter. This will be done in light of the most recent gravity experiment data and radio occultation measurements from the Juno spacecraft, as well as the latest zonal wind measurements obtained with the Hubble Space Telescope and James Webb Space Telescope.

How to cite: Fonsetti, M., Caruso, A., Zannoni, M., Tortora, P., Galanti, E., Kaspi, Y., and Smirnova, M.: Geodetic Modeling of Gas Giants: An Integrated Approach Applied to Jupiter, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16961, https://doi.org/10.5194/egusphere-egu25-16961, 2025.

EGU25-16985 | ECS | Posters on site | PS7.2

Experimental Study of Image Matching Techniques for Co-Registration and Data Fusion of Orbital and Ground-Based Planetary Images 

Antonia Schriever, Klaus Gwinner, Patrick Irmisch, Thomas Kraft, and Jörg Brauchle

This study aims to investigate the potential and feasibility of multi-sensor image integration to combine images from orbital or airborne platforms with rover-based images in planetary exploration. We use images taken with the airborne Modular Aerial Camera System (MACS) and a hand-held camera, the Integrated Positioning System (IPS), on a steep hillside on Vulcano Island, Sicily. Typical use-cases in planetary exploration are for robotic navigation, localization of exploration targets or improved target coverage combining additional viewpoints.

MACS was operated on a Vertical Take-Off and Landing (VTOL) drone. The images were used to simulate the orbital images overflying the hillside, while the IPS images were used to simulate a ground-based platform (e.g. rover). The aerial images were taken at a constant height level, resulting in different distances to the ground due to elevation changes in the terrain. The IPS images are taken with a 16mm lens camera mounted diagonally upwards relative to the other sensors on the system. The hillside is captured along a path that is approximately parallel to the steep scarp, maintaining a distance of at least 100 meters from it. Images are taken at multiple stops always covering the whole hillside with a swivel movement. This simulates different stereo angles to experiment with later during 3D reconstruction. The resulting dataset includes images from two different sensors with a high viewpoint discrepancy. We evaluate the performance of image matching when using this dataset regarding among other things varying scales, resolution and wavelength. Also, we investigate terrain specific influences on the matching quality as well as methods to overcome the viewpoint discrepancy between MACS and IPS images, resulting in large image parallaxes and local variation of the difference in image resolution. Lastly, we evaluate the quality of resulting 3D reconstruction as well as of the estimated intrinsic and extrinsic camera parameters and the possibility for their improvement.

We compare the results to earlier tests based on orbital planetary images, using various different matching methods. An evaluation with focus on feature-based matching approaches was done on images coming from the High Resolution Stereo Camera (HRSC) on ESA’s MarsExpress mission [1, 2]. Multiple performance metrics were analyzed which showed that different methods excel under different criteria. Also, it emphasized the need for a certain richness in features to ensure precise and accurate points. A majority of feature detectors reach subpixel accuracy, but only in feature rich images, while cross-correlation points as input to least-squares matching (LSM) [3] outperform otherwise.

[1] Schriever, A. and Gwinner, K., EPSC 2024, DOI: 10.5194/epsc2024-986

[2] Jaumann, R., et al. PSS 55 (7–8), 928–952 (2007) DOI: 10.1016/j.pss.2006.12.003.

[3] Gwinner, K., et al. PE&RS 75(9), 1127-1142 (2009), DOI 10.14358/PERS.75.9.1127

How to cite: Schriever, A., Gwinner, K., Irmisch, P., Kraft, T., and Brauchle, J.: Experimental Study of Image Matching Techniques for Co-Registration and Data Fusion of Orbital and Ground-Based Planetary Images, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16985, https://doi.org/10.5194/egusphere-egu25-16985, 2025.

EGU25-17253 | Orals | PS7.2

Seismic Instrument for Asteroids (SIA): a seismometer based on geophone sensors for the RAMSES mission to Apophis 

Alexandre Cadu, Raphael Garcia, Naomi Murdoch, Joe De Martini, Anthony Sournac, Arnaud Wilhelm, Pauline Carpi, David Mimoun, Taichi Kawamura, Philippe Lognonné, Patrick Michel, and Pierre Bousquet

The internal structure of small asteroids (diameter < 1 km) remains poorly known, and recent spacecraft/surface interactions performed by the Osiris-REX and Hayabusa2 missions produced unexpected results about their physical properties.

What is the level of macro- and micro-porosity? What are the cohesive forces? Are the bodies stratified, heterogeneous or more homogenous? The answers to these questions have strong implications for both the long-term evolution of these bodies and for planetary defense.

Seismology experiments on such objects are difficult due to the low gravity and the possible small amount of natural seismic sources on these objects. However, during its pass close to the Earth in 2029, seismic activity will be generated in the asteroid Apophis by tidal stresses. This unique opportunity of natural seismic sources is exploited by the SIA instrument concept, which is planned to be deployed to the surface of the asteroid by the ESA RAMSES mission before the close encounter of Apophis with the Earth.

We first present and justify both the science case and the concept of operations of the seismic measurements on Apophis during the close encounter with the Earth. We then describe the instrument itself by presenting the current development status and system budgets. Finally, we discuss the lander platform requirements to reach the seismometer measurement performances and the science objectives.

How to cite: Cadu, A., Garcia, R., Murdoch, N., De Martini, J., Sournac, A., Wilhelm, A., Carpi, P., Mimoun, D., Kawamura, T., Lognonné, P., Michel, P., and Bousquet, P.: Seismic Instrument for Asteroids (SIA): a seismometer based on geophone sensors for the RAMSES mission to Apophis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17253, https://doi.org/10.5194/egusphere-egu25-17253, 2025.

EGU25-17634 | Orals | PS7.2

Deep space weather radio observations of JUICE spacecraft with VLBI radio telescopes 

Guifre Molera Calves, Oliver White, Jasper Edwards, Giuseppe Cimo, Dominic Dirkx, Luigi Gisolfi, and Vidhya Pallichadath

The Jupiter Icy Moons Explorer (JUICE), launched by the European Space Agency on April 14th, 2023, is on an eight-year journey to the Jovian system, arriving in July 2031. Among its eleven experiments, the Planetary Radio Interferometric and Doppler Experiment (PRIDE) stands out conduction Earth-based radio measurements. PRIDE leverages a network of Very Long Baseline Interferometry (VLBI) radio telescopes worldwide to perform radio science experiments [Gurvits 2023]. These experiments include radio occultation studies of Jupiter’s atmosphere, monitoring space weather, and precisely determining the dynamics of the JUICE spacecraft, and the ephemerides of Jupiter and its moons. For instance, these ephemerides are essential for understanding the long-term orbital and interior evolution of the icy moons, shedding light on their tidal interactions and geological history.

The University of Tasmania (UTAS) plays a role in this mission through its operation of a continent-wide network of five large radio telescopes: Hobart-12m, Katherine-12m, Yarragadee-12m, Hobart-26m, and Ceduna-30m. Since 2010, these telescopes have been used for planetary tracking by conducting radio science experiments to support missions such as Venus Express, Mars Express, and BepiColombo [Molera Calves 2021]. During the 2023-2024 period, UTAS’s VLBI radio telescopes have been actively monitoring the X-band radio downlink signals from various spacecraft, including Mars Express, Tianwen-1, BepiColombo, Solar Orbiter, and JUICE [Kummamuru 2023, Maoli 2023, Noor 2025 and Edwards 2025]. These observations are particularly valuable during solar conjunctions, when the spacecraft are aligned with the Sun, allowing for precise measurements of the solar corona. In addition, several we have reported and studied the transit of Coronal Mass Ejections (CMEs) across the radio propagation path. These observations provide estimates of the propagation and velocities of CMEs, enhancing our ability to forecast space weather events and their potential impacts.

How to cite: Molera Calves, G., White, O., Edwards, J., Cimo, G., Dirkx, D., Gisolfi, L., and Pallichadath, V.: Deep space weather radio observations of JUICE spacecraft with VLBI radio telescopes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17634, https://doi.org/10.5194/egusphere-egu25-17634, 2025.

EGU25-17955 | ECS | Posters on site | PS7.2

The Radio Science Experiment on Hera, Juventas and Milani 

Edoardo Gramigna, Paolo Tortora, Riccardo Lasagni Manghi, Marco Zannoni, Ryan S. Park, Giacomo Tommei, Sebastien Le Maistre, Daniel J. Scheeres, Michael Kueppers, and Patrick Michel

Hera, the European Space Agency’s pioneering planetary defense mission, was successfully launched on October 7, 2024, from Cape Canaveral aboard a SpaceX Falcon 9 rocket. This milestone marks a critical step in the Asteroid Impact and Deflection Assessment (AIDA) collaboration, which Hera undertakes in synergy with NASA’s DART mission. The mission's primary objective is to perform an in-depth post-impact analysis of the Didymos binary asteroid system, focusing on Dimorphos, the smaller moon that served as DART’s impact target.

Hera’s investigations aim to evaluate the effectiveness of the kinetic impactor technique as a method for asteroid deflection, while also providing critical insights into the physical and compositional characteristics of Dimorphos. These findings will not only refine our understanding of asteroid behavior under kinetic impact but also contribute to developing strategies for planetary defense against potential future asteroid threats.

Central to Hera’s scientific approach is its advanced radio science experiment. This includes an X-band radio link, which supports high-precision Earth-based two-way range and range-rate measurements, alongside Delta-Differential One-Way Ranging (Delta-DOR) observations. Additionally, the mission leverages inter-satellite ranging between Hera’s main spacecraft and its two CubeSats, Juventas and Milani, complemented by optical navigation imaging and altimetry data. Together, these techniques will significantly enhance the accuracy of Hera's data and allow for a more comprehensive reconstruction of the impact event and its aftermath.

This work provides a summary of the Hera radio science experiment investigation, the experimental framework and operational plans during its cruise phase and its close-proximity operations at the Didymos system. Furthermore, it discusses the expected scientific outcomes of Hera’s radio science experiment, emphasizing its pivotal role in advancing planetary defense capabilities and contributing to the broader goals of asteroid science.

How to cite: Gramigna, E., Tortora, P., Lasagni Manghi, R., Zannoni, M., Park, R. S., Tommei, G., Le Maistre, S., Scheeres, D. J., Kueppers, M., and Michel, P.: The Radio Science Experiment on Hera, Juventas and Milani, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17955, https://doi.org/10.5194/egusphere-egu25-17955, 2025.

EGU25-18084 | Posters on site | PS7.2

 COSPAR Panel on Exploration (PEX) Exploration Roadmap: The Case for Mars 

Heather Smith, Michel Blanc, and Andre Galli

The new phase of exploration offers multiple perspectives, for the space community and for many other sectors of activity. But it also brings some threats to the preservation of scientific research and environmental stewardship of Mars. A proactive integration of environmental awareness into the new wave of  exploration will be the best way to mobilize public and private stakeholders, federate their resources and their creativity, and preserve for future generations the natural environment of Mars. The new wave of robotic and sample return from Mars will hopefully take place in an era of increased environmental awareness for our own planet, in which close monitoring of environmental impacts of human activities will drive innovative solutions to mitigate them

In this presentation we describe land-use and management policies by various countries and U.S. Agencies in an effort to balance environmental preservation, resource utilization and economic interests.   In particular we compare the U.S federal land management system and ecotourism policies with preservation of natural landscapes and resource use. We describe the Mars Sample return re-re-design concepts from the eight selected teams with regard to sustainable exploration of Mars. 

How to cite: Smith, H., Blanc, M., and Galli, A.:  COSPAR Panel on Exploration (PEX) Exploration Roadmap: The Case for Mars, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18084, https://doi.org/10.5194/egusphere-egu25-18084, 2025.

EGU25-18169 | ECS | Orals | PS7.2

Cassini Bistatic Radar Campaign during the Prime and Equinox Missions: Heterogeneous Reflections from Titan's Solid Surfaces 

Giancorrado Brighi, Valerio Poggiali, Marco Mastrogiuseppe, Marco Zannoni, Alexander Hayes, and Paolo Tortora

During the Cassini Prime (2004-2008) and Equinox (2008-2010) missions, the Radio Science Subsystem onboard the Cassini spacecraft conducted seven bistatic radar (BSR) observations of Titan, Saturn’s largest moon. A variety of terrains, including unique geological features such as plains and dunes identified by the Cassini RADAR, were observed across equatorial, mid-latitude, and south-polar regions.

In this radio science experiment, Cassini’s High-Gain Antenna (HGA) transmitted unmodulated, right-hand circularly polarized signals at three frequencies—S-band (λ=13 cm), X-band (λ=3.6 cm) and Ka-band (λ=0.94 cm)—toward Titan’s surface. The antenna was pointed to enable quasi-specular reflections from the illuminated portion of the moon’s surface to be received by NASA’s Deep Space Network (DSN) antennas on Earth, which have the capability to receive both left-hand and right-hand circularly polarized components of the reflected signals. The investigation of quasi-specular echoes, when detectable, can provide constraints on surface roughness and near-surface effective dielectric constant, which is connected to the structural and compositional properties of Titan’s terrains.

Analysis of the BSR data from these seven experiments reveals highly heterogeneous scattering behavior across Titan’s surface. Reflections range from barely detectable signals, characterized by broad, diffuse echoes just above the noise floor, to narrower and more powerful reflections suggesting the presence of very smooth and isolated patches of land. Such heterogeneity in surface scattering was also noticed during ground-based observations of Titan by means of the Green Bank Telescope and Arecibo Observatory.

In this work, we present a detailed analysis of this largely unexploited dataset, highlighting regional variations in forward scattering and providing preliminary findings about surface roughness and near-surface dielectric constant of various regions on Titan. Whenever possible, we compare the BSR findings with Cassini SAR maps of Titan’s surface and discuss correlations between scattering variations observed by the two instruments.

How to cite: Brighi, G., Poggiali, V., Mastrogiuseppe, M., Zannoni, M., Hayes, A., and Tortora, P.: Cassini Bistatic Radar Campaign during the Prime and Equinox Missions: Heterogeneous Reflections from Titan's Solid Surfaces, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18169, https://doi.org/10.5194/egusphere-egu25-18169, 2025.

EGU25-18455 | Orals | PS7.2

Enhancing Lunar Exploration: Drilling, Sensing, and Sampling Systems for In-Situ Regolith Subsurface Analysis and for Sample Return 

Lutz Richter, Ranjan Prabhat, Kumar Dinesh, Shubhro Chakrabartty, and Tze Ng

We report on the development of two promising analysis and sampling tools for use on the Moon that promise to enhance science return in upcoming lunar missions and which would inform the search for potentially valuable resources that would be worthwhile exploiting. Building on the success of ISRO's Chandrayaan missions, our efforts aim at 1) creating an advanced drilling instrument with an integrated sensing unit, referred to as the “Moon Sensing Drill" (MSD), and 2) a “Soil and Pebble Sampler” (SPS). The MSD partially builds on concepts already studied in Europe under an “instrumented drill" heading whereas the SPS is entirely new. We are realizing the systems in collaboration between D Y Patil International University in Pune, India, and European entities.

The MSD would be able to drill autonomously into lunar regolith and analyze the subsurface column in real-time, including detection of 3He, volatiles and key minerals. Moreover, temperature and thermal conductivity sensors would be part of the drill. The design is based primarily on a percussive drilling system, with the sensors incorporated inside the drill stem. The sensor data will be sent wirelesslessly to an electronics unit that integrates the information. This way, no rotary transmission of signal cables to and from sensors needs to be incorporated into the drill. Power transmission to the sensors is however via slip rings. The system can either be carried on a lunar rover or on lander Maximum drilling depth into the regolith is 20 cm. We are currently designing and building a demonstrator.

The Soil Pebble Sampler (SPS) is a versatile tool designed to allow the collection and analysis of soil / regolith and pebble samples. In particular, the SPS is the first ever concept for uncrewed missions for controlled sampling of both soil and pebbles in a single tool. This will be key to future sample return missions to the Moon, such as Chandrayaan-4 in the ISRO space program.

In the case of Drilling Mode, SPS employs a rotary drill equipped with radial blades and an external, thin-walled auger to drill into soil. With progressing depth, a longitudinal cavity (“tunnel") incorporated in the drill stem is filled with regolith. One of the SPS assemblies is the ball-end vibrating mechanism, which is able to shake particles loose from the drill and therefore keep debris from becoming lodged in the drill tip and the associated samples. Moreover, the vibrating mechanism is essential in shaking out the soil that would have been pressed into the sample tunnel.

A stable 3-jaw gripping structure is at the end of the ball-end vibrating mechanism and uses that mechanism's sideways motion capability to pick up a pebble.

How to cite: Richter, L., Prabhat, R., Dinesh, K., Chakrabartty, S., and Ng, T.: Enhancing Lunar Exploration: Drilling, Sensing, and Sampling Systems for In-Situ Regolith Subsurface Analysis and for Sample Return, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18455, https://doi.org/10.5194/egusphere-egu25-18455, 2025.

EGU25-18991 | Orals | PS7.2

Cassini-Huygens bistatic experiment from Titan's surface 

Miguel Pérez-Ayúcar

After a successful entry and descent on Titan, on 14 January 2005, the probe remarkably survived the landing and continued radioing from the surface to the overflying Cassini, until the orbiter set below Titan’s local horizon.

The inter probe-satellite Huygens to Cassini sinal provided, other than the communications functionality, an unanticipated bistatic radio scattering experiment from Titan’s surface. This the our knowledge the furthest bistatic link experiment established between two spacecrat to date.

In the paper we summarize the high-quality measurements of the 2098 MHz (14.3 cm) postlanding radio signal, focusing on the variations observed in signal strength. The mechanism that creates this pattern is physically interpreted as multipath interference between the direct signal and the signal reflected on Titan’s surface.

A roughness property of pebble sizes in the order of 10cm is finally derived. It should be noted that this measurement is in a completely new direction from the after-landing cameras fixed view, complementing the surface knowledge of the Huygens landing area.

How to cite: Pérez-Ayúcar, M.: Cassini-Huygens bistatic experiment from Titan's surface, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18991, https://doi.org/10.5194/egusphere-egu25-18991, 2025.

EGU25-19429 | ECS | Posters on site | PS7.2

The LUMIO Radio Science Experiment 

Riccardo Lasagni Manghi, Giancorrado Brighi, Davide Banzi, Luis Antonio Gomez Casajus, and Fabio Ferrari

The European Space Agency mission LUMIO (Lunar Meteoroid Impacts Observer) aims to characterize the lunar and near-Earth meteoroid environment by imaging impact flashes on the far side of the Moon. During its 1-year operative phase along a quasi-periodic Halo orbit about the Earth-Moon Lagrangian point L2, LUMIO will observe the lunar far side while keeping its line of sight to the Earth unobstructed. With this geometry, the LUMIO spacecraft may be the first miniaturized satellite to exploit its radio communication system to carry out bistatic radar observations of the near-limb regions of the Moon, which may help characterize the surface roughness and dielectric constant around recent impact sites. Furthermore, high-frequency VIS-NIR images collected by the LUMIO-Cam during science operations represent an opportunity for testing innovative orbit determination techniques, such as using precise timing of stellar occultations to complement ground-based radiometric measurements. Stellar occultation measurements are expected to improve the navigation accuracy during science observation windows, aiding in absolute positioning of the impact sites and reducing the reliance on ground tracking. This work will outline the proposed LUMIO Radio Science Experiment, its main objectives, and expected performances, highlighting the potential of bistatic radar observations and stellar occultations to enhance the characterization of lunar impact flashes.

How to cite: Lasagni Manghi, R., Brighi, G., Banzi, D., Gomez Casajus, L. A., and Ferrari, F.: The LUMIO Radio Science Experiment, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19429, https://doi.org/10.5194/egusphere-egu25-19429, 2025.

EGU25-19903 | Orals | PS7.2

Mass Determination of the Lucy Mission target asteroids using radio tracking data 

Matthias Hahn, Martin Paetzold, Tom Andert, Harold Levison, Keith Noll, and Simone Marchi

The LUCY spacecraft was launched in 2021. After two gravity assists at Earth and the flybys at binary main-belt asteroid (152830) Dinkinesh in November 2023 and just recently at (52246) Donaldjohanson in the asteroid belt the spacecraft is now on its way to characterize several trojan asteroids. These outer solar system asteroids are located in the Lagrange points L4 and L5 of the Jupiter-Sun system.

The first flyby will be at (3548) Eurybates and its moon Queta in August 2027, followed directly by the flyby at (15094) Polymele with its moon Shaun (informal name) in September 2027. Two more flybys in the so-called Greek camp in the L4 point are at (11351) Leucus in April 2028 and at (21900) Orus in November 2028. After orbiting the Sun once more the spacecraft will reach the L5 swarm of asteroids and will flyby at the binary system of (617) Patroclus and Menoetius in March 2033.

During these flybys the mass of the target asteroids shall be determined using the Doppler tracking method. Analytic solutions for the error estimation of the mass determination have already shown that the required precision will be met. However, this analytic approach does not take into account several error sources like time limited tracking, no Doppler data +/- 2h around closest approach, uncertainties in the initial spacecraft position and velocity for a flyby, non-gravitational forces, etc. Another contributing error source is the Doppler noise imposed on the signal. Doppler data from ESAs Rosetta mission and NASAs New Horizons spacecraft as well as tracking data recorded during the first 3 1/2 years of LUCYs cruise phase could be analyzed regarding distance, solar wind turbulence, integration times etc. A numeric orbit determination using simulated Doppler data can provide the most realistic error estimation using all perturbing forces and uncertainties. A detailed analysis of the error of the mass determination for all flybys shall be presented.

How to cite: Hahn, M., Paetzold, M., Andert, T., Levison, H., Noll, K., and Marchi, S.: Mass Determination of the Lucy Mission target asteroids using radio tracking data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19903, https://doi.org/10.5194/egusphere-egu25-19903, 2025.

EGU25-20037 | Orals | PS7.2

A novel ENA instrument for Space Weather monitoring: SWEATERS (SWEATERS-Space WEATher Ena Radiation Sensors) project 

Elisabetta De Angelis, Alessandro Mura, Federico Pilo, Paolo Maestro, and Stefano Orsini and the SWEATERS team

SWEATERS (Space WEATher Ena Radiation Sensors) project has the purpose to realize an innovative ENA sensor for Space Weather application and plasma monitoring.

ENA (Energetic Neutral Atoms) signal detection is a well proven technique able to provide information about Solar wind interaction with planetary environments providing plasma global imaging. 

SWEATERS sensor is a new ENA instrument concept based for the first time on gas detector technique. The challenge of the project is to apply advanced particle detection technologies developed in the HEP field to instruments for space application, e.g. ENAs in space.

The MicroMegas gas detector (MM) developed at CERN is the baseline for this new ENA sensor concept. The main advantage is to provide all the requested items of ENA detection (mass, energy, direction) in a unique and compact system.

Sensors installed on a cluster of platforms orbiting at low altitude around the Earth could provide new detailed information on the plasma populations generated in perturbation phenomena.

How to cite: De Angelis, E., Mura, A., Pilo, F., Maestro, P., and Orsini, S. and the SWEATERS team: A novel ENA instrument for Space Weather monitoring: SWEATERS (SWEATERS-Space WEATher Ena Radiation Sensors) project, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20037, https://doi.org/10.5194/egusphere-egu25-20037, 2025.

EGU25-20361 | Orals | PS7.2

Sniffing the Enceladus Plume: The High Ice Flux Instrument (HIFI) Compositional Analyzer 

Sascha Kempf, Micheal Creager, Scott Tucker, Zoltan Sternovsky, Sean Hsu, Morgan Cable, Libor Nouzak, Bernd Abel, and Frank Postberg

The Cosmic Dust Analyzer (CDA) on the Cassini spacecraft has convincingly demonstrated the scientific value of mass spectra of ice particles ejected by the plume on Saturn's ice moon Enceladus. Trace amounts of organic and inorganic molecules embedded in ice particles revealed invaluable insight into the chemical composition of the ocean beneath the moon's icy crust. However, it became quickly obvious that to address open questions about the astrobiological nature of the ocean requires impact ionisation mass spectrometers with a considerably higher mass resolution than that of the CDA instrument of m/Δm ~ 50. Other CDA shortcomings include target cleanliness issues and the low detection cadence of 1 impact per second.

 

The High Ice Flux Instrument (HIFI) is a reflectron-type impact mass spectrometer specifically designed for such applications. It has a mass resolution of 1000 to 2000 and has been optimized for using the electronics of the Surface Dust Analyser instrument on Europa Clipper for recording the spectra. To ensure a high mass resolution HIFI has a long drift region and uses a set of electrostatic Einzel lenses to prevent the ion beam from diverging before entering the single stage reflectron region. The reflectron optics is composed of 23 precision machined electrostatic electrodes to guarantee a smooth reflecting field. In contrast to previous reflectron impact mass spectrometers such as CIDA enter the impacting particles the spectrometer through the reflectron to strike the target at a right angle. The target itself is a highly polished Titanium carrier coated with 250 nm of high purity Iridium (nm surface roughness). The high atomic mass of Iridium ensures that no target lines as well as target cluster lines appear in the mass range ≤ 200 u relevant for the compositional analysis of mineral and ice particles.

The instrument performance has been verified through the impact of metal particles at high velocities. Additionally, experiments were conducted with ice particles to illustrate the capacity of HIFI to discern minute quantities of salts and organics in the spectra of water ice.

How to cite: Kempf, S., Creager, M., Tucker, S., Sternovsky, Z., Hsu, S., Cable, M., Nouzak, L., Abel, B., and Postberg, F.: Sniffing the Enceladus Plume: The High Ice Flux Instrument (HIFI) Compositional Analyzer, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20361, https://doi.org/10.5194/egusphere-egu25-20361, 2025.

EGU25-20702 | ECS | Posters on site | PS7.2

Design and Development of multiple space particle energy spectrum analyzer 

Chih-Yu Chiang, Tzu-Fang Chang, Tzu-EN Yen, Yung-Tsung Cheng, Cheng-Tien Chen, Yu-Rong Cheng, Sheng-Cheng Tsai, Pei-Ying Kuo, Chien-Hui Chan, Po-Jui Li, Ping-Ju Liu, and Tsung-Pin Hung

The multiple space particle spectrum analyzer has been proposed as the scientific payload of the Formosat-8C satellite (FS-8C). This multiple space particle energy spectrometer is a small, low-weight, low-power consumption advanced analyzer. Its design was originally derived from the STE (Supra Thermal Electron) detector on the STEREO satellite. This analyzer uses an evolved a multi-channel detector component, which can measure electrons and ions in the energy range of approximately 1 ~ 200 keV, and can establish high-energy neutral atom imaging, hoping to provide information to the space science community more valuable data. The prototype of this payload has been initially produced, and it can comply with the overall interface specifications of the FS-8C, including a size of < 2U, a weight of < 5kg, an average orbital power consumption of less than 2W. We expect to complete the delivery of the flying model in September 2026 according to the schedule.

How to cite: Chiang, C.-Y., Chang, T.-F., Yen, T.-E., Cheng, Y.-T., Chen, C.-T., Cheng, Y.-R., Tsai, S.-C., Kuo, P.-Y., Chan, C.-H., Li, P.-J., Liu, P.-J., and Hung, T.-P.: Design and Development of multiple space particle energy spectrum analyzer, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20702, https://doi.org/10.5194/egusphere-egu25-20702, 2025.

EGU25-20719 | Posters on site | PS7.2

Development of the All-Sky Electrostatic Analyzer for a Lunar Rover 

Tzu-Fang Chang, Chih-Yu Chiang, Sheng-Cheng Tsai, Yu-Rong Cheng, Tzu-En Yen, Zhao-Yu Huang, Chien-Hui Chan, Cheng-Tien Chen, Po-Jui Li, Ping-Ju Liu, Yung-Tsung Cheng, Pei-Ying Kuo, Tsung-Pin Hung, Yu-Ting Lyu, Cheng-Lin Tsai, Shiuan-Hal Shiu, Jih-Run Tsai, and Shin-Fa Lin

All-Sky Electrostatic Analyzer (A-ESA) is a scientific payload that will be mounted on a lunar rover and is designed to observe the variations of plasma environment on the Moon. A-ESA is composed of an electrostatic analyzer on the top, and an MCP assembly, power supply units and electronics are located under it. A-ESA has the entrance scanning deflectors and the inner scanning deflectors. The entrance of A-ESA is electrically scanned within ~90∘in vertical direction, i.e. A-ESA has hemi-spherical field of view (FOV). When A-ESA is operating in observation mode, the collection of science data is divided into 8 parts in horizontal direction and 6 parts in vertical direction. And it generates 16 energy levels via sweeping high voltage. Therefore it can measure the plasma distribution function and charged particle energy in hemi-sphere space on the lunar surface. Since the launch of the science payload project, PDR, CDR, TRR and PAR reviews have been completed. Now we are carrying out function tests and performance tests. Initial function tests between A-ESA and the lunar rover have been performed too. At the end of 2024, the A-ESA has been delivered to Taiwan Space Agency (TASA).

How to cite: Chang, T.-F., Chiang, C.-Y., Tsai, S.-C., Cheng, Y.-R., Yen, T.-E., Huang, Z.-Y., Chan, C.-H., Chen, C.-T., Li, P.-J., Liu, P.-J., Cheng, Y.-T., Kuo, P.-Y., Hung, T.-P., Lyu, Y.-T., Tsai, C.-L., Shiu, S.-H., Tsai, J.-R., and Lin, S.-F.: Development of the All-Sky Electrostatic Analyzer for a Lunar Rover, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20719, https://doi.org/10.5194/egusphere-egu25-20719, 2025.

EGU25-20977 | Orals | PS7.2

Instrument Design Updated of the Venus Emissivity Mapper (VEM) for VERITAS and Envision 

Yaquelin Miriam Rosas Ortiz and the team Venus Emissivity Mapper (VEM) for VERITAS and Envision

The Venus Emissivity Mapper (VEM) is a groundbreaking instrument designed to transform our understanding of Venus. Developed for NASA’s VERITAS and ESA’s EnVision orbiters, this advanced push-broom multispectral imager is tailored to reveal the planet’s surface. VEM features a 14-band filter assembly, an InGaAs detector with thermoelectric cooling, a turn-window mechanism, and a dual-stage baffle system to ensure performance in Venus's harsh environment. Weighing just 6 kilograms, it will achieve over 70% global coverage, enabling unprecedented surface mapping. VEM promises to unveil Venus's secrets and deepen our understanding of Earth’s enigmatic sister planet.

 

Optics: The VEM/VenSpec-M Optics (VEMO), developed by CNES and LESIA, uses a telecentric 3-lens system for precision imaging. Its entrance lens focuses the Venusian scenery onto a filter assembly, while relay optics with <1 magnification transfer the image to a 16.4 mm focal length detector. With a 46.4° field of view, it achieves a 207 km swath width at a 250 km orbit. The filter assembly (0.86–1.18 µm), developed by Bertin Winlight and CILAS, maps the image across 14 filter stripes, enabling surface emission measurements and atmospheric corrections.

Detector: The VEM detector features an InGaAs short-wave infrared sensor with an integrated thermoelectric cooler, eliminating the need for a cryocooler. Qualified for space, it undergoes rigorous environmental testing. The detector covers 400–1700 nm (optimized to 790–1510 nm), with 640 x 512 pixels at a 20 µm pitch, operating from -40°C to +70°C (baseline 0°C). Its quantum efficiency peaks at ~85%, aligning with the VEM spectral range. System-level analyses show signal-to-noise ratios around 100, even at the mission's end, with a margin exceeding 100%. While a radiation test campaign is complete, managing increased dark current from proton irradiation remains a challenge.

Testing and Analysis: A thermal cycling test was conducted as part of the evaluation campaign on two flight-representative sealed detectors following the MIL-STD-883 standard (method 1010, condition A). The temperature range was adjusted to -43°C to -40°C and +85°C to +88°C, staying within the detector’s non-operative limits. The test involved 100 cycles with a 125°C total range achieved in 16 minutes, resulting in a gradient of approximately 8°C per minute. A follow up of the structural analysis has been performed showing that the loads at the VEMO interface are higher than initially expected, resulting in increased loads at the detector level. The engineering team will explore potential solutions, including updates to the mechanical design to mitigate the loads. 

Keywords: VERITAS, VEM, EnVision, VenSpec-M, Venus, IR, N-IR, SWIR, InGaAs, Imaging

Acknowledgments: CNES/LESIA for its contribution on the optics development.

How to cite: Rosas Ortiz, Y. M. and the team Venus Emissivity Mapper (VEM) for VERITAS and Envision: Instrument Design Updated of the Venus Emissivity Mapper (VEM) for VERITAS and Envision, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20977, https://doi.org/10.5194/egusphere-egu25-20977, 2025.

GI4 – Earth Observation systems & instrumentation from remote to proximal sensing

Terrestrial laser scanning (LiDAR) and photogrammetry are a recent innovation in spatial information data acquisition, which allows geological outcrops to be digitally captured with unprecedented resolution and accuracy. With point precisions and spacing of the order of a few centimetres, an enhanced quantitative element can now be added to geological fieldwork and analysis, opening up new lines of investigation at a variety of scales in all areas of field-based geology. Integration with metric imagery allows 3D photorealistic models to be created for interpretation, visualization and education.

The studied pillow lavas belong to the Middle Volcano-Sedimentary Formation in Western Srednogorie magmatic region. More than ten lava flows of this type have been identified.

3D models provide the opportunity to draw conclusions about the conditions of formation of aqueous flows. One of the factors controlling the growth of the pillow lavas is cooling rate. This can be determined through the analysis and measurements of the thickness and distinctiveness of the quenched (peripheral) rims of every individual lava lobes. Well-defined and distinct rims indicate relatively rapid cooling rates. The morphology and size of separate pillows largely depend on the basins slope angle on which the lava flowed. Their morphology is also influenced by the effusion rate and lava viscosity. The formation of large and rounded pillow obes is typical for moderate slope angles.

The application of terrestrial laser scanning (LiDAR) and photogrammetry enables the precise and detailed digital capture of geological outcrops, significantly enhancing field-based geological studies. In the case of pillow lavas from the Middle Volcano-Sedimentary Formation in the western Srednogorie magmatic region, these technologies allow for the creation of 3D photorealistic models, which aid in interpreting the conditions under which the lavas formed. Key factors influencing the growth and morphology of pillow lavas include cooling rates, slope angles, effusion rates, and viscosity. Rapid cooling produces well-defined quenched rims, while moderate slopes favor the development of large, rounded pillow lobes. These insights provide a deeper understanding of the dynamics of subaqueous lava flows and their formation processes.

How to cite: Velev, S.: LiDAR and photogrammetry technology and its application in paleovolcanic reconstructions of pillow lavas. A case study from Western Srednogorie, Bulgaria., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3067, https://doi.org/10.5194/egusphere-egu25-3067, 2025.

EGU25-3082 | ECS | Posters on site | GI4.1

Development of Low-Cost Instrumentation for Comprehensive Global Ocean Monitoring 

Juan Francisco Martinez-Osuna, Viviana Piermattei, Riccardo Valentini, Francesco Renzi, Giovanni Coppini, and Marco Marcelli

The high costs associated with traditional marine research instruments remain a significant barrier to conducting detailed studies, limiting the granularity and availability of oceanographic data. This directly affects the analysis of complex phenomena such as the impacts of human activities and climate change on coastal zones, which are particularly vulnerable to sea level variations, flash floods, and storm surges. These events, capable of causing irreversible damage, demand real-time monitoring with high spatial resolution to understand their evolution and mitigate their impacts. Furthermore, large-scale monitoring of marine species is crucial to better understand their behavior and distribution areas, providing valuable information for the conservation and management of marine ecosystems.

To address these limitations, we propose the development of a low-cost, robust, precise, and easy-to-implement instrumentation, ideal for citizen science projects. Our approach is based on a versatile, low-power data acquisition module built around the STM32L microcontroller. This module includes ports for connecting various sensors, as well as remote data transmission, geolocation, and memory storage capabilities. Its versatile design makes it suitable for a wide range of applications.

This work presents two innovative applications of this technology. The first innovation is a low-cost tide gauge based on ultrasonic sensors, designed to accurately measure water levels in seas and rivers. This device can integrate with early warning systems, facilitating the monitoring of changes in water levels and providing fundamental data to assess the impacts of climate change on marine ecosystems and coastal communities. The second is a new tracking device (TAG) for marine fauna, designed to gather key information about distribution areas, habitat use, and species behavior in relation to the physical and biogeochemical characteristics of the water column. This TAG incorporates, among other features, a multispectral sensor that enables the study of water quality and composition, as well as the monitoring of Photosynthetically Active Radiation (PAR) at different depths.

How to cite: Martinez-Osuna, J. F., Piermattei, V., Valentini, R., Renzi, F., Coppini, G., and Marcelli, M.: Development of Low-Cost Instrumentation for Comprehensive Global Ocean Monitoring, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3082, https://doi.org/10.5194/egusphere-egu25-3082, 2025.

EGU25-4350 | Posters on site | GI4.1

Next generation modular processing system for miniaturized remote sensing instruments 

Georg Schardt, Tom Neubert, Heinz Rongen, Egon Zimmermann, Thomas Gulde, Erik Kretschmer, Guido Maucher, Jörn Ungermann, Peter Preusse, Martin Riese, and Ghaleb Natour

The study of climate-relevant processes in the atmosphere using airborne platforms is an important contribution to understanding our environment. The deployment of remote sensing instruments on aircraft or balloons requires powerful computer systems for data acquisition and instrument control. The ongoing trend towards further miniaturisation of instruments, with increasingly complex measurement tasks and higher data rates for use over longer flight durations, requires a new generation of control and processing units. These units must be significantly reduced in mass, volume and power consumption. In addition, a shift in data management from storage and post-processing to real-time data processing is required to reduce the increasing amounts of data and to transmit them to ground stations.

Based on years of experience with the GLORIA (Gimballed Limb Observer for Radiance Imaging of the Atmosphere) instrument and its current miniaturised version, GLORIA-Lite, a modular and reconfigurable data acquisition and processing platform has been developed. This platform is specifically designed to meet the demanding requirements of future long-duration flights in harsh environments, with significant optimisations in weight, volume and power consumption. Using state-of-the-art multi-processor system-on-chip (MPSoC) modules, the platform enables real-time data processing while significantly reducing the need for data storage or transmission. Redundancy in hardware and software using the multiple processor cores, together with a supervisor circuit, makes the platform ready for harsh environments. Thanks to its compact form factor, the ruggedised and fully reprogrammable hardware is adaptable to a wide range of applications, further enhancing its versatility and potential for use in various scientific and technological missions.

This presentation will show the prototype of the new processing platform, which will be used together with the GLORIA-Lite instrument during an upcoming balloon campaign. First processing steps and performance analysis will be presented.

How to cite: Schardt, G., Neubert, T., Rongen, H., Zimmermann, E., Gulde, T., Kretschmer, E., Maucher, G., Ungermann, J., Preusse, P., Riese, M., and Natour, G.: Next generation modular processing system for miniaturized remote sensing instruments, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4350, https://doi.org/10.5194/egusphere-egu25-4350, 2025.

EGU25-5591 | Posters on site | GI4.1

Soil management and branch position influence wine grape physiology: insights from TreeTalkers data on sap flow 

Gabriele Pizzileo, Simone Beltramino, Alessandra Nuzzo, Valentina Scardigno, and Maria Vincenza Chiriacò

Optimizing soil management practices in vineyards is essential for enhancing grapevine resilience under climate change conditions. This study, funded by the Italian PNRR AGRITECH project, exploits low-cost sensors (TreeTalkers) to evaluate the effects of different soil management practices on sap flow density and crop yield across the annual growth cycle, particularly under heat stress conditions,  defined as temperatures exceeding 35°C. Real-time sensors allowed monitoring of physiological and environmental parameters in two plots of a controlled vineyard environment, comparing conventional tillage vs no-tillage with spontaneous cover crops used as mulch. Data were analyzed based on temperature thresholds and branch position. Results from the TreeTalkers are presented into a visualization platform and indicate a significant correlation between soil management practices and sap flow density at high temperatures,  highlighting the benefits of no-tillage and mulching in mitigating the effects of heat stress and enhancing grapevine resilience against heat waves,  an increasingly pressing issue in the Mediterranean region. Furthermore, no significant differences in sap flow density or yield were observed between lower and upper branches, suggesting uniform physiological performance across plant structures. This study highlights the importance of integrating real-time low-cost technologies to promote sustainable viticulture and broader Earth observation applications.

How to cite: Pizzileo, G., Beltramino, S., Nuzzo, A., Scardigno, V., and Chiriacò, M. V.: Soil management and branch position influence wine grape physiology: insights from TreeTalkers data on sap flow, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5591, https://doi.org/10.5194/egusphere-egu25-5591, 2025.

EGU25-6061 | Posters on site | GI4.1

Closing coastal and marine observation gaps thanks to cost-effective solutions 

Peter Thijsse, Tjerk Krijger, Dick Schaap, Emilie Breviere, Patrick Gorringe, and Antonio Novellino

Traditional coastal and marine monitoring methods are often costly and resource-intensive. In order to make observations more affordable and accessible to a wider range of users, the global collaborative initiative ’Solutions for Cost-effective Ocean Observation Platform’ (SCOOP) was designed. SCOOP aims to connect cost-efficient device developers, data managers, data collectors and users (scientists, researchers, citizen scientists…) to encourage collaboration and enhance the collection and sharing of marine data. SCOOP is an open-access web-platform (https://scoop-ocean.org/) providing access to a comprehensive catalogue of low-cost sensors and emerging technologies, and a series of documentation and expertise for users to help them optimize their data collection and management practices. SCOOP wants to ensure that collected data adheres to FAIR (Findability, Accessibility, Interoperability, Reusability) principles, facilitating its integration into global data infrastructures. SCOOP was endorsed by the UN Decade of Ocean Science for Sustainable Development in 2024 and is supported by developments in several European and global initiatives (EMODnet, JERICO, GOOS, Synchro and CoastPredict).

A direct example of the potential is provided by the EU-funded LandSeaLot project running since 2024 until 2028. LandSeaLots main objective is to make big steps in closing observation gaps in the land-sea interface, focusing on river deltas. By integrating in situ, model, and Earth Observation (EO) data, LandSeaLot connects key communities and initiatives such as Copernicus, ESA, EEA, GEOSS, EMODnet, and the European Digital Twin of the Ocean. The project focuses on improving observation capabilities, reducing gaps between models and observations, and enhancing data integration from sensors, satellites, and models. A key component of the project is the deployment of low-cost sensors, guided by citizen scientists through networks like TransEurope Marinas. These sensors will be tested in the LandSeaLot Integration Labs (LILs) across strategically selected regions across Europe which have diverse catchment, tidal, and meteorological conditions. These LILs will integrate improved observation techniques, providing data for tackling societal challenges such as carbon fluxes, plastic transfer, nutrient impacts, eutrophication, biodiversity conservation, and climate change adaptation. To support international data interoperability and make the data FAIR, LandSeaLot will analyse the deployment protocols, as well as data and metadata models, and have close communication with the developers for adjustments at the source. With input from cost-effective devices developers, users and data managers, and with LandSeaLot results, SCOOP will be further implemented to promote and democratise the use of cost-effective sensors and devices in oceanography and beyond.

How to cite: Thijsse, P., Krijger, T., Schaap, D., Breviere, E., Gorringe, P., and Novellino, A.: Closing coastal and marine observation gaps thanks to cost-effective solutions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6061, https://doi.org/10.5194/egusphere-egu25-6061, 2025.

EGU25-9921 | ECS | Posters on site | GI4.1

Automating Phenological Stage Detection from Citizen Science Images for Plant Phenology Monitoring 

Negin Katal, Michael Rzanny, Susanne Tautenhahn, Patrick Mäder, Hans Christian Wittich, David Boho, and Jana Wäldchen

Plant phenology, the study of seasonal events in plants' life cycles such as budburst, flowering onset, leaf-out, fruit ripening, and senescence, is intrinsically linked to climatic conditions and plays a crucial role in ecosystem processes like carbon and nutrient cycling. Due to its ecological importance, many countries have established phenological monitoring networks based on systematic protocols. However, declining volunteer participation in recent decades has raised concerns about the continuity of these invaluable datasets.

Advancements in technology, machine learning, and smartphone accessibility have spurred the development of plant identification apps. These apps enable users to identify plant species without prior botanical knowledge, generating vast datasets of plant occurrences.

This study investigates the potential of applying machine learning to citizen science-derived plant image data for phenological monitoring. By utilizing a pre-trained deep learning model, we extracted relevant image features and classified 39 species-specific phenostages for nine common plant species in Germany using a Support Vector Machine (SVM) classifier. Our model achieved an impressive overall accuracy of 96%, enabling the automated annotation of over 600,000 plant occurrence images from the Flora Incognita app into corresponding phenological stages.

With this approach, not only did we capture additional fine-granular phenostages, such as flower bud and unripe fruit stages, which are less commonly resolved in traditional phenological network datasets, but we also observed the interannual variability of each phenostage across different years. This demonstrates the feasibility of integrating opportunistic citizen science data into phenological monitoring schemes. By addressing the challenges posed by declining volunteer participation, this method significantly enhances the temporal and spatial resolution of phenological datasets, offering innovative opportunities for phenology monitoring and ecological research.

How to cite: Katal, N., Rzanny, M., Tautenhahn, S., Mäder, P., Wittich, H. C., Boho, D., and Wäldchen, J.: Automating Phenological Stage Detection from Citizen Science Images for Plant Phenology Monitoring, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9921, https://doi.org/10.5194/egusphere-egu25-9921, 2025.

The advancement of low-cost instrumentation is a critical development to ensure the longevity of ocean observing systems and the sustainability of marine environmental studies. This topic represents one of the most innovative trends in contemporary oceanographic research, aligning with the 2030 Agenda and supporting the objectives of the Global Ocean Observing System (GOOS).
These instruments must be developed with a focus on modularity to serve diverse purposes, including vertical profiling, stand-alone systems, and deployment on various platforms such as buoys, Voluntary Observing Ships, and underwater vehicles. The accessibility of affordable technologies enables the establishment of extensive observational networks, facilitating the study of marine physical and biogeochemical processes through an integrated approach combining in situ measurements, predictive modeling, and remote sensing data.
This study introduces newly developed low-cost sensors and probes designed to measure key oceanographic parameters, including temperature, conductivity, chlorophyll a, and Chromophoric Dissolved Organic Matter (CDOM) fluorescence. These developments build upon the electronic redesign of the T-FLAP and subsequent technologies created within the LOSEM framework (e.g., Marcelli et al., 2015; Piermattei et al., 2018; Marcelli et al., 2021). These instruments underwent rigorous testing during multiple oceanographic surveys conducted in the Mediterranean Sea, yielding valuable insights into their performance and potential for large-scale deployment in marine research.

How to cite: Marcelli, M. and Madonia, A.: Development of a modular probe to measure CTD and Chlorophyll a fluorescence for multipurpose oceanographic applications, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10313, https://doi.org/10.5194/egusphere-egu25-10313, 2025.

EGU25-11464 | ECS | Posters on site | GI4.1 | Highlight

Crop Talker: An Innovative IoT Solution for Multispectral and Structural Monitoring in Small-Scale Agriculture 

Valerio Coppola, Francesco Renzi, FIlippo Tagliacarne, and Riccardo Valentini

Efficient monitoring of crop health and growth dynamics is essential for sustainable agricultural practices, particularly in small-scale farming systems. The Crop Talker represents a breakthrough in precision agriculture as a multifunctional, low-cost Internet of Things (IoT) device. Integrating advanced sensing technologies, it provides comprehensive ecophysiological insights.

Key features include a 28-band spectrometer covering the 400–900 nm range for assessing physiological parameters such as nitrogen content, chlorophyll levels, and nutrient deficiencies. Additionally, the Crop Talker incorporates an 8×8-pixel Lidar Time-of-Flight (ToF) sensor to deliver real-time crop height measurements, augmented by RGB imaging from a 2 MP camera for visual assessments. Onboard environmental sensors for air temperature and humidity complement the system, enabling holistic crop monitoring. Data streaming is facilitated through a 4G NB-IoT connection, ensuring seamless integration with remote analytical platforms.

This innovative device is designed to empower smallholder farmers by delivering actionable insights through an affordable and robust monitoring tool. The Crop Talker bridges the gap between traditional farming practices and modern digital agriculture, contributing to enhanced crop management and resource efficiency.

How to cite: Coppola, V., Renzi, F., Tagliacarne, F., and Valentini, R.: Crop Talker: An Innovative IoT Solution for Multispectral and Structural Monitoring in Small-Scale Agriculture, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11464, https://doi.org/10.5194/egusphere-egu25-11464, 2025.

EGU25-11676 | Posters on site | GI4.1

A visualization platform for TreeTalkers data: supporting sustainable vineyard practices 

Alessandra Nuzzo, Valentina Scardigno, Simone Beltramino, Maria Vincenza Chiriacò, and Gabriele Pizzileo

The ability to analyze and visualize (near) real-time data is crucial for addressing the challenges posed by climate change in agriculture. This work presents a data visualization system for TreeTalker sensors, funded by the Italian PNRR AGRITECH project, which monitors sap flow density and environmental parameters in vineyards. By providing user-friendly access to sensor data, the system enhances decision-making in soil management and grapevine physiology studies.
Featuring an intuitive web-based interface, the platform processes raw sensor outputs into interactive dashboards, allowing users to explore the effects of soil management practices, such as conventional tillage versus no-tillage with mulching, on grapevine resilience under heat stress. Key functionalities include dynamic environmental filtering, comparative plot analyses, and the ability to assess branch-specific physiological responses. Additionally, the system supports temporal tracking of sap flow variations across the growing season.
By converting complex datasets into actionable insights, the system enables researchers and/or vineyard managers to adopt data-driven approaches for sustainable viticulture. This tool demonstrates the potential of low-cost, scalable technologies and advanced visualization techniques to promote sustainable practices in agriculture, with broader applicability beyond viticulture.

How to cite: Nuzzo, A., Scardigno, V., Beltramino, S., Chiriacò, M. V., and Pizzileo, G.: A visualization platform for TreeTalkers data: supporting sustainable vineyard practices, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11676, https://doi.org/10.5194/egusphere-egu25-11676, 2025.

EGU25-15337 | Posters on site | GI4.1

Dual-Transmission Oceanographic Buoy : A Low-Cost Solution for Accessible Coastal Monitoring 

Nicola Madonia, Juan Francisco Martinez Osuna, Francesco Renzi, Valerio Coppola, and Marco Marcelli

The development of efficient and cost-effective instruments for marine monitoring is crucial for advancing the collection of oceanographic data. This paper introduces a novel, low-cost, multipurpose oceanographic drifter-buoy designed to provide reliable, high-resolution data acquisition in both coastal and offshore environments. Engineered to enhance marine observations while maintaining affordability, the drifter achieves an optimal balance between cost and functionality by utilizing readily available components.

The drifter features a spherical body equipped with a solar panel to recharge its battery pack, enabling sustainable and long-term operations. It incorporates water temperature and turbidity sensors, with data acquisition and processing managed by an ARM® Cortex®-M0+ microcontroller. Position tracking is achieved through GNSS technology, ensuring precise geolocation.

To ensure reliable communication, the drifter is equipped with dual systems: LoRa technology for nearshore data transmission via gateways and Globalstar satellite communication for offshore data transmission. Its modular design further allows the integration of additional sensors, supporting a wide range of applications.

The dual communication system guarantees uninterrupted data transmission to the server regardless of the drifter’s position. All acquired data will be visualized and made freely available for download via the European Marine Observation and Data Network (EMODnet). Furthermore, these measurements will support environmental monitoring and the validation of numerical models to simulate coastal physical and biological processes at high spatial and temporal resolution.

With its dual communication system, solar-powered design, robust data acquisition capabilities, and cost-efficiency, this drifter-buoy represents a versatile, accessible, and sustainable tool for oceanographic monitoring and coastal observation systems.

How to cite: Madonia, N., Martinez Osuna, J. F., Renzi, F., Coppola, V., and Marcelli, M.: Dual-Transmission Oceanographic Buoy : A Low-Cost Solution for Accessible Coastal Monitoring, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15337, https://doi.org/10.5194/egusphere-egu25-15337, 2025.

EGU25-15462 | Posters on site | GI4.1

Tetraspec: a new low-cost spectrometer for ecosystem monitoring applications 

Alice Madonia, Marco Marcelli, Francesco Renzi, Valerio Coppola, and Riccardo Valentini

Environmental monitoring is essential in enhancing our understanding of natural ecosystems functioning, addressing effective responses to the challenges posed by climate change, pollution and biodiversity loss. The Internet of Things technology (IoT) has significantly improved observing capabilities, enabling continuous and real-time data collection, even from remote locations, thereby extending the spatial and temporal coverage of environmental monitoring systems. A major challenge still lies in acquiring in situ optical data, which are essential for improving assessments of primary production rates as well as of marine food web dynamics, carbon cycling processes and ecosystem resilience.

Featuring high-quality components, modularity and low power consumption, Tetraspec technology, developed by Nature 4.0, is a 28-channels spectrometer that operates over a range of 410 nm to 940 nm and includes measurements of Photosynthetically Active Radiation (PAR) and Near-Infrared (NIR). Tetraspec is a low-cost, portable and accurate system capable of acquiring a great amount of data for remote sensing and numerical models validation, being easily integrated with various acquisition systems.

This work presents the results of the Tetraspec's laboratory and in situ calibration, detailing its optical characteristics, operational capabilities and applications in both terrestrial and marine environments, through the comparison with reference standard instruments.

 

How to cite: Madonia, A., Marcelli, M., Renzi, F., Coppola, V., and Valentini, R.: Tetraspec: a new low-cost spectrometer for ecosystem monitoring applications, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15462, https://doi.org/10.5194/egusphere-egu25-15462, 2025.

EGU25-15736 | Posters on site | GI4.1

Challenges, Opportunities and Lessons learnt of Low-Cost Open-Source and DIY Initiatives in Coastal Oceanography 

Alex Herrada, Joan Puigdefàbregas, Gabriel Jordà, Eider Loyola, Manel Grifoll, Benjamí Calvillo, Joan Villalonga, and Damià Gomis

The need for comprehensive and sustained coastal oceanographic monitoring has grown as climate change, pollution, and human activities increasingly impact marine ecosystems. Traditional monitoring systems, while highly accurate and reliable, are often prohibitively expensive, limiting their accessibility to resource-constrained regions and organizations. Low-cost/open-source (LoCOs) and do-it-yourself (DIY) initiatives have emerged as promising alternatives, leveraging accessible materials, open-source technology, and community engagement to democratize data collection.

In this presentation, we explore the challenges, opportunities and lessons learnt associated with such initiatives through several examples in the Western Mediterranean Sea and Mozambique coastal waters. In those regions, and for the last 10 years, oceanographic field campaigns, coastal monitoring networks and citizen science initiatives have been launched using DIY and LoCos devices measuring waves, sea level, surface velocities, water temperature and bathy-topographies.

The experience gained during this decade has given us enough elements to discuss challenges involved with this type of technology. This includes ensuring data accuracy and standardization, system durability in harsh marine environments, and overcoming technical knowledge barriers among non-specialist users. Also, this technology opens new opportunities, including fostering citizen science, enabling localized and high-resolution monitoring, and promoting capacity-building in underserved regions. Finally, we will discuss up to what extent low-cost/open-source and DIY solutions have the potential to revolutionize coastal monitoring, offering scalable and sustainable pathways for managing and conserving marine environments.

How to cite: Herrada, A., Puigdefàbregas, J., Jordà, G., Loyola, E., Grifoll, M., Calvillo, B., Villalonga, J., and Gomis, D.: Challenges, Opportunities and Lessons learnt of Low-Cost Open-Source and DIY Initiatives in Coastal Oceanography, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15736, https://doi.org/10.5194/egusphere-egu25-15736, 2025.

EGU25-19116 | ECS | Posters on site | GI4.1

Design and Implementation of a Low-Cost Edge-Computing Gateway for LoRaWAN Networks 

Filippo Tagliacarne, Riccardo Valentini, Francesco Renzi, and Valerio Coppola

As the Internet of Things (IoT) continues to grow, efficient and reliable communication methods are essential for enabling widespread connectivity, particularly in remote and resource-constrained environments. LoRa, with its low power consumption and long-range capabilities, has become a cornerstone of IoT communication. The LoRaWAN protocol extends this functionality by enabling devices to transmit data globally through internet-connected gateways. These gateways aggregate data packets from nearby devices and forward them to centralized servers.
However, traditional LoRaWAN gateways face significant limitations. They are often cost-prohibitive, require constant internet connectivity, and lack advanced data processing capabilities, making them unsuitable for deployment in areas with unreliable or no cellular coverage. These limitations hinder the adoption of LoRaWAN in scenarios such as environmental monitoring and rural IoT networks.
To address these challenges, we developed a low-cost, energy-efficient edge-computing LoRaWAN gateway using embedded systems such as Raspberry Pi 0. Unlike conventional gateways, these edge-computing gateways locally process incoming data, enabling intelligent features such as optimized transmission, data buffering during network outages, and adaptive communication strategies. Additionally, these gateways can be configured to operate independently of cellular networks by utilizing satellite connectivity, further enhancing their usability in remote or off-grid applications.
Preliminary testing demonstrates that these gateways consume up to one-third of the power required by traditional gateways while maintaining reliable data transmission. This substantial reduction in power consumption extends operational lifespans and reduces deployment costs. The ability to process and optimize data locally also improves network efficiency, ensuring timely and reliable communication even under challenging conditions.
This innovation provides a scalable, cost-effective solution for IoT connectivity in remote and underserved regions. By addressing the limitations of conventional gateways, these edge-computing gateways enhance the feasibility of deploying IoT networks in scenarios where traditional infrastructure is impractical or unavailable. The broader implications of this work include improved access to IoT technologies for applications such as environmental monitoring and agriculture, ultimately expanding the reach and impact of IoT systems worldwide.

How to cite: Tagliacarne, F., Valentini, R., Renzi, F., and Coppola, V.: Design and Implementation of a Low-Cost Edge-Computing Gateway for LoRaWAN Networks, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19116, https://doi.org/10.5194/egusphere-egu25-19116, 2025.

EGU25-19284 | Posters on site | GI4.1

Fishing Vessel Ocean Observing Network: An Emerging Collaborative Global Network 

Patrick Gorringe, Cooper Van Vranken, Christopher Cusack, António Miguel Piecho-Santos, Michela Martinelli, Carles Castro Muniain, Hassan Moustahfid, Moninya Roughan, and Julie Jakoboski

Integrated multidisciplinary ocean observations are critical for understanding ocean processes and supporting robust climate- and ocean-related forecasts, which inform sustainable fisheries management, adaptation strategies that reduce risk, and increased coastal resilience. However, subsurface oceanographic and biogeochemical data is scarce in coastal, shelf, and boundary regions due to the challenges of deploying traditional free-drifting ocean observing platforms in these dynamic environments. 

Coastal areas are vital for fishing. Therefore, not only do fishing activities coincide with spatio-temporal ocean data gaps, but fishing vessels serve as platforms for a range of oceanographic instruments, and many types of fishing gear already profile the water column. By eliminating the two largest cost components of ocean observing (the platform and deployment of that platform), innovative sensors can gather valuable subsurface data along the ride at a fraction of the cost. An example of this approach is given by the Moana project, in which a cost-effective smart sensor was deployed on fishing gear to automatically download a thermal profile even on vessels with limited power and electronics. Approximately 250 vessels reversed the coastal data gaps created by the Argo program’s success in the open oceans and demonstrated substantial error-reducing capabilities in high-resolution regional ocean models. Similarly, a compact ferrybox-type style flow-through system is used in Portugal to continuously measure temperature, salinity, chlorophyll, Dissolved Oxygen (DO), pH, Oxidation-Reduction Potential (ORP), and turbidity. 

This approach is intrinsically inclusive as cost-effective sensors increase accessibility in historically underserved regions and non-traditional stakeholders are empowered to improve sustainability, profitability, and resilience in their own communities. Data from the Environmental Monitors on Lobster Traps and Large Trawlers (eMOLT) Program is used in the American lobster (Homarus americanus) stock assessment and improves forecasts for US Coast Guard search and rescue operations. The Moana Project provided analyses and ocean forecasts of coastal circulation, marine heatwaves, and connectivity to New Zealand’s seafood industry and other stakeholders. The AdriFOOS (Adriatic Fishery and Oceanography Observing System) Program is one of the longest-running programs to use fishing boats for the collection of scientifically-useful datasets. Fishers directly benefit from these data streams as exemplified by the Smart Fisheries Network (SFiN) led by Kyushu University (Japan), which assimilates CTD and ADCP data from over 200 vessels into coastal ocean models that enable participating fishers to operate both more safely and efficiently. Sensors have additionally been installed on a range of artisanal and industrial vessels across Ghana, The Bahamas, Tanzania, the Bering Sea, and Australia. 

To maximize these benefits and democratize ocean observation, the Fishing Vessel Ocean Observing Network (FVON) is an emerging network within the Global Ocean Observing System that coordinates common standards for technology and deployment, establishes best practices, standardizes data flows, and facilitates observation uptake across programs. Through these activities, FVON seeks to achieve its mission: to foster collaborative fishing vessel-based observations, improve ocean predictions and forecasting, promote sustainable fishing practices, and facilitate a data-driven blue economy. 

How to cite: Gorringe, P., Van Vranken, C., Cusack, C., Piecho-Santos, A. M., Martinelli, M., Castro Muniain, C., Moustahfid, H., Roughan, M., and Jakoboski, J.: Fishing Vessel Ocean Observing Network: An Emerging Collaborative Global Network, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19284, https://doi.org/10.5194/egusphere-egu25-19284, 2025.

EGU25-19999 | Posters on site | GI4.1

Advancing Ecosystem Service Quantification with a Low-Cost Soil Box Technology forAgroecological Systems 

Riccardo Valentini, Nicole Cecchinato, Simona Castaldi, Maria Vincenza Chiriaco, Valerio Coppola, and Francesco Renzi

Quantifying ecosystem services (ES) is essential for evaluating the sustainability of agricultural systems,
particularly in agroecological contexts where practices such as reduced tillage, cover cropping, and crop
diversification aim to enhance soil health, biodiversity, and carbon storage. However, current methods for ES
assessment often rely on expensive, labor-intensive, or destructive sampling approaches, limiting their
accessibility and scalability across both research and practical land management contexts. To address this
gap, we present a novel, low-cost soil box system designed for real-time, multi-parameter monitoring of
ecosystem services in agricultural soils.
The soil box integrates a network of advanced yet cost-effective sensors capable of capturing physical (e.g.
moisture content, temperature), chemical (e.g. N-P-K, SOC, TOC), and biological indicators (e.g. microbial
activity) in real time. Technologies such as microbial biosensors, CO₂ flux sensors, NIR spectroscopy, and
ATP detectors enable continuous, non-destructive measurements across multiple soil layers. Its modular
design allows for scalable deployment across experimental plots, long-term monitoring trials, and on-farm
applications, making it highly versatile for both scientific research and practical land management for
farmers.
The ability to capture a diverse range of ES indicators in situ also reduces the need for costly external
laboratory analyses, minimizing logistical barriers often associated with large-scale monitoring efforts.
Therefore, the soil box system has the potential to revolutionize how ecosystem services are measured and
understood in agricultural systems. Its real-time, high-resolution data can inform both sustainable
agricultural practices and scientific research, providing robust evidence of agroecological benefits for soil
health, carbon sequestration, and biodiversity conservation. This aligns directly with the objectives of the
European Green Deal and CAP reforms, offering a scalable, evidence-based tool for assessing the impact of
agricultural practices on ecosystem health, climate resilience, and long-term productivity.
Keywords: agroecology, ecosystem services, soil monitoring, low-cost technology, carbon storage, real-time data,
sustainable agriculture, participatory research.

How to cite: Valentini, R., Cecchinato, N., Castaldi, S., Chiriaco, M. V., Coppola, V., and Renzi, F.: Advancing Ecosystem Service Quantification with a Low-Cost Soil Box Technology forAgroecological Systems, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19999, https://doi.org/10.5194/egusphere-egu25-19999, 2025.

The Rural Revitalization Strategy is a major initiative launched by China to address the emerging challenges facing agriculture and rural areas under new historical conditions. Geographical elements such as the human-environment relationship, resource distribution, and physical geography are closely linked to the all-round development of the countryside, providing a theoretical basis for the implementation of the rural revitalization strategy, while mapping geographic information data, as an important support for rural revitalization, plays an irreplaceable role in precise policymaking and scientific planning. Among various remote sensing observation means and earth observation instruments, unmanned aerial vehicle (UAV) technology has seen rapid advancement due to its high spatial resolution, flexibility, and cost-effectiveness, revealing significant potential for rural revitalization research. At EGU25, we will present the innovative applications of UAV data across multiple rural revitalization scenarios. Specifically, we will discuss the use of UAV data in rural industrial development, illustrated by marine aquaculture in coastal towns; the role of UAV data in preserving historical and cultural heritage; its contribution to urban-rural integration and governance in urban villages; and the promising future of UAV data in rural tourism development, including digital tourism and 3D navigation. Additionally, we will outline methods for processing multi-sensor UAV data and demonstrate how these results are integrated into practical platforms to foster rural development. We hope that this exchange will inspire broader applications of drone technology in rural development worldwide, contributing to the comprehensive and sustainable advancement of global rural areas.

How to cite: Kuang, J.: Innovative Applications of UAV Data in Rural Revitalization: Case Studies and Insights, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-588, https://doi.org/10.5194/egusphere-egu25-588, 2025.

EGU25-1708 | Posters on site | GI4.2

Improving FAIRness of drone data through community effort 

Alice Fremand, Sarah Manthorpe, Mari Whitelaw, Jens Klump, and Thabo Semong

The use of Uncrewed Aerial Vehicles (UAVs), including both autonomous and remotely piloted aerial systems, is increasingly prevalent across various scientific disciplines, enabling the collection of large volumes of data for diverse research applications. These data are essential for environmental monitoring, such as terrestrial and marine studies, species detection, and atmospheric data collection. However, the volume of data generated and the absence of standardised workflows often complicate data sharing and publication. To address these challenges, the Natural Environment Research Council (NERC) Environmental Data Service (EDS, [1]) has developed guidelines aimed at ensuring that UAV-collected data are Findable, Accessible, Interoperable, and Re-usable (FAIR) [2][3]. In collaboration with the Research Data Alliance, ongoing efforts are focused on developing recommendations for both general and domain-specific data formats and metadata, while also addressing challenges such as ethics and the use of persistent identifiers (PIDs) for instruments [4]. These efforts aim to streamline the data lifecycle for research using small UAVs and autonomous platforms, facilitating integration into research cloud infrastructures.

 

 [1] https://eds.ukri.org/environmental-data-service

[2] Fremand, Alice. 2023 UAV data management handbook. UK Polar Data Centre, British Antarctic Survey, 13pp. https://nora.nerc.ac.uk/id/eprint/536392/

[3] Fremand, Alice. 2023 Towards a data commons: Imagery and derived data from autonomous and remotely piloted aerial vehicles. UK Polar Data Centre, British Antarctic Survey, 24pp. https://nora.nerc.ac.uk/id/eprint/536398/

[4] https://www.rd-alliance.org/groups/small-uncrewed-aircraft-and-autonomous-platforms-data-working-group/members/all-members/

How to cite: Fremand, A., Manthorpe, S., Whitelaw, M., Klump, J., and Semong, T.: Improving FAIRness of drone data through community effort, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1708, https://doi.org/10.5194/egusphere-egu25-1708, 2025.

EGU25-1818 | Posters on site | GI4.2

Estimation of Photovoltaic Capacity and Detection of Gully Erosion based on Drone-generated 3D Terrain Models. 

Yu Cheng Kuo, Sin Ting Lin, and Yu Shen Hsiao

In recent years, the frequency of extreme climate events has increased, and global warming has intensified. The growing occurrence and severity of such events have prompted nations to place greater emphasis on carbon emission reduction and environmental protection. Concurrently, the rapid depletion of traditional energy sources, coupled with rising global energy demand, has made the development of renewable energy a critical priority. Among the various renewable energy sources, solar photovoltaics (PV) has emerged as a highly promising solution due to its clean and efficient characteristics. As flat land resources become increasingly limited in certain regions, sloping terrains are increasingly being considered as viable sites for solar PV installations, owing to their favorable sunlight exposure and land utilization potential. However, the installation and maintenance of PV systems on slopes present several challenges, including low inspection efficiency, high operational costs, and risks to the structural stability of the systems, which are exacerbated by slope-specific geological hazards such as erosion. This study proposes an integrated approach for hotspot identification and erosion detection in photovoltaic (PV) systems installed on sloped terrains using drone technology. By utilizing drone-derived 3D terrain models, the study estimates actual solar illumination and detects disaster-inducing erosion gullies within potential PV installation zones, thereby facilitating the identification of optimal installation sites. The results of this research will serve as a critical reference for the deployment of PV systems in complex terrains, with particular emphasis on assessing the associated slope disaster risks.

How to cite: Kuo, Y. C., Lin, S. T., and Hsiao, Y. S.: Estimation of Photovoltaic Capacity and Detection of Gully Erosion based on Drone-generated 3D Terrain Models., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1818, https://doi.org/10.5194/egusphere-egu25-1818, 2025.

EGU25-1821 | Posters on site | GI4.2

Research on Seamless 3D Modeling Using UAV Technology Combined with Smartphone LiDAR 

Sin Ting Lin, Yu Cheng Kuo, and Yu Shen Hsiao

In recent years, the rise of the "digital twin" concept has significantly expanded the potential applications of 3D modeling in disaster prevention engineering. Among these, unmanned aerial vehicle (UAV) technology has emerged as a key method for terrain and structural modeling. As UAV technology continues to advance rapidly, its use in engineering has become increasingly widespread. With their high mobility and low-altitude operational capabilities, UAVs effectively overcome challenges such as post-disaster traffic disruptions and cloud cover. They are now widely utilized in tasks like terrain mapping, regional inspections, vegetation seeding, and disaster prevention surveys. Despite these advantages, UAV-based 3D modeling faces challenges. Vegetation often obstructs the clear capture of structures, and modeling resolution can be inadequate for certain applications. However, the LiDAR functionality integrated into smartphones offers a promising solution. This technology enables the rapid creation of high-precision 3D models and the accurate measurement of structural dimensions and volumes, even in steep terrains or remote locations that are difficult to access. This study explores the integration of UAV technology with ground-based LiDAR scanning using the iPhone 15 Pro, aiming to achieve seamless 3D modeling through an air-ground integration approach. The research focuses on merging aerial and ground point clouds. To accomplish this, we will employ both commercial software (e.g., Pix4Dmatic) and custom-developed point cloud fusion techniques. Each approach will be evaluated and compared comprehensively in terms of cost, processing time, and model accuracy. By combining UAV with smartphone-based applications, this study is expected to significantly improve model accuracy and detection efficiency in disaster prevention engineering. Moreover, the proposed approach holds broad potential for application in other fields, such as road design, landscape architecture, and urban planning.

How to cite: Lin, S. T., Kuo, Y. C., and Hsiao, Y. S.: Research on Seamless 3D Modeling Using UAV Technology Combined with Smartphone LiDAR, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1821, https://doi.org/10.5194/egusphere-egu25-1821, 2025.

EGU25-3114 | Posters on site | GI4.2

Hyperspectral UV-Vis Reflectance Imaging Using UAVs for Leaf Area Index Remote Sensing 

Tomasz Berezowski, Marcin Kulawiak, and Marek Kulawiak

Although ultraviolet (UV) reflectance is linked to various environmental factors, it remains underutilized in remote sensing applications. This study explores the potential of UV-visible (UV-vis) reflectance for vegetation monitoring using unmanned aerial vehicles (UAVs). A UAV-mounted spectrometer was employed to collect point reflectance data across the study area, which was then georeferenced and interpolated to produce continuous reflectance images. The leaf area index (LAI) was used to illustrate the effectiveness of UV reflectance in vegetation monitoring. Our findings indicate strong agreement between UAV-derived reflectance images and Sentinel-2 data. Validation revealed that incorporating UV reflectance into LAI models alongside visible reflectance resulted in an R² improvement of up to 29.2% and an RMSE reduction of up to 18.9%, compared to models using only visible reflectance. This study demonstrates that UV reflectance measurements in the 320–400 nm range are feasible with UAV-based remote sensing and that hyperspectral UV-vis reflectance imaging offers significant value for vegetation monitoring. Additionally, the results suggest that refining our measurement system or performing experiments in a different environment could enable reflectance measurements at wavelengths as low as 290 nm.

How to cite: Berezowski, T., Kulawiak, M., and Kulawiak, M.: Hyperspectral UV-Vis Reflectance Imaging Using UAVs for Leaf Area Index Remote Sensing, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3114, https://doi.org/10.5194/egusphere-egu25-3114, 2025.

EGU25-6139 | Posters on site | GI4.2

Creating Digital Twins of Mountain Complex Terrains: A Study Case in the Lazaun Rock Glacier, South Tyrol, Italy 

Abraham Mejia-Aguilar, Giovanni Dedivitiis, Chiara Crippa, Giovanni Cuozzo, Matteo Delpero, Raul-David Serban, Stefano Brighenti, Giacomo Marrazzo, and Francesco Calvetti

A Digital Twin (DT) is an accurate virtual representation of a physical object, phenomenon, or process. DTs are utilized in geosciences to simulate and analyze complex terrains. Developing DTs of rock glaciers is essential due to their significant role in addressing challenges related to climate change, monitoring permafrost, water resource management, and the dynamics of mountain ecosystems. Creating a DT of a rock glacier is very challenging because of the monitoring strategy (regarding spatial, temporal, and spectral resolution), the selected tools for processing, analyzing, and simulating data collected, and the computational infrastructure.  

In this work, we study the rock glacier of Lazaun, South Tyrol, Italy (southern Ötztal Alps). The actively moving rock glacier (elevation range 2,480 to 2,700 m a.s.l.; 0.12 km2) is a prominent site for long-term monitoring and research, being one of the most investigated rock glaciers worldwide in terms of internal structure, motion, and hydrological behaviour.

Here, we present a scale-down strategy starting from remote sensing products using differential synthetic aperture radar interferometry (DInSAR) to analyze extensive areas and identify active zones. Over these identified zones, we introduced a proximal sensing approach using drones equipped with specialized sensors.

Using high-resolution cameras, we captured and combined overlapping images through photogrammetry techniques to generate detailed orthomosaics, 3D models, and Digital Surface Models. Additionally, we incorporated thermal imaging from UAV sensors to detect land surface temperature variations, inspect the presence of subsurface ice, and identify areas of activity.

These data sources offer unparalleled spatial resolution and detail, which is crucial for building an accurate DT. Using GNSS to determine displacement and velocity, we continued a long-lasting in-situ method to measure the coordinates of specific features (boulders). We integrate ground photography to identify their shapes in drone products for further automatic shape identification.

Finally, we introduced the use of FLAC3D (Fast Lagrangian Analysis of Continua for 3D modeling) to understand the propagation and evolution of the rock glacier movement by using a viscous constitutive model whose parameters have been calibrated by matching the velocity field of the central part of the glacier. We propose the use of Azure Digital Twins tool to visualize the possible combinations of data and scenarios. 

How to cite: Mejia-Aguilar, A., Dedivitiis, G., Crippa, C., Cuozzo, G., Delpero, M., Serban, R.-D., Brighenti, S., Marrazzo, G., and Calvetti, F.: Creating Digital Twins of Mountain Complex Terrains: A Study Case in the Lazaun Rock Glacier, South Tyrol, Italy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6139, https://doi.org/10.5194/egusphere-egu25-6139, 2025.

EGU25-7590 | ECS | Posters on site | GI4.2

UAV Mapping and AI Recognition for Inspection of Structural Defects in Water Resources 

Yi-Hsuan Kan, Guan-Jyun Jiang, and Jen-Yu Han

To increase the efficiency and accuracy of traditional hydraulic construction inspections, this study proposes an automated inspection and data management system using UAV and artificial intelligence (AI) technology. A 600-meter-long part of the river was chosen as a demonstration area, with emphasis on the use of bank condition study and deterioration identification. The approach consists of three major components. Initially, high-resolution photographs were obtained by drone once a month. Second, the YOLOv8 and Unet++ models were used to segment and detect damage in the photos. Finally, a data management platform was developed to allow for the systematic integration of picture data and the automated compilation of standardised inspection reports. The results indicate that the strategy considerably improves inspection efficiency and accuracy. The combination of uav and AI technology greatly reduces inspection time and successfully inspects a 600-meter radius of the bank. The model achieves a high IOU score and several damage detection indexes in berm segmentation, demonstrating the technical solution's practicality and application promise. This study confirms the potential use of UAV and AI technologies for hydraulic structural inspection, offering an efficient and data-driven inspection solution. Future research will focus on improving the AI model's performance, broadening the range of data samples, and supporting the complete implementation of intelligent monitoring and maintenance of water conservancy infrastructure.

How to cite: Kan, Y.-H., Jiang, G.-J., and Han, J.-Y.: UAV Mapping and AI Recognition for Inspection of Structural Defects in Water Resources, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7590, https://doi.org/10.5194/egusphere-egu25-7590, 2025.

EGU25-17148 | Posters on site | GI4.2

4D Digital Twin geological modelling for sustainable quarry management 

Jose Kullberg, Ricardo Pereira, Ana Machadinho, and Alexandre Santos

Exploitation of ornamental rock from quarries requires innovative approaches that can provide sustainable access to construction materials. Within a quarry, rock types can vary significantly, and its assessment demands a detailed evaluation of its lithological variations and fracture network. Adequate resource management is critical to minimize product waste, improve process efficiency and increase its worth along the value chain.

Using Unmanned Aerial Vehicles (UAVs), operating at low level flights, equipped with high resolution RGB cameras, GPS and GNSS systems, in addition to real-time differential data (RTK) and GCP, image datasets were acquired to perform 4D reconstructions and interpret highly detailed morphologic and geologic features.

We report the results of rock typing obtained from Digital Elevation Models, Orthophotos, Point Clouds and Mesh datasets, such as fracture network characterization and cavity delineation, that provide essential information about penalizing features, mandatory for informed decision-making during exploitation. These include: 1) manual and automated fracture delineation; 2) rock typing; 3) optimization of the exploitation plan, 4) volumetric estimation of land and karst cavities; and 5) stock management.

We used segmentation techniques on point clouds to analyze structural discontinuities and identify faults and fractures at different scales, in the quarry extraction fronts. The applied algorithms enable the automatic extraction of geological planes and determine the geometric characteristics of the point cloud. The RGB color variation in the point clouds was also analyzed, enabling the delimitation of areas with different colors, which are generally associated with the degree of rock alteration. This analysis also allows the accurate detection of fracture networks. Results from image analysis allow individualising discrete types of rock and confidently extract fracture networks. The discrete features extracted from the models were subsequently validated with fieldwork at the quarries.

Acknowledgements: The authors thank Research Project PRR - Sustainable Stone by Portugal integrated on the Mobilizing Agenda and Fundação para a Ciência e a Tecnologia, I.P. (FCT), Portugal, through the research unit UIDB/04035/2020 - GeoBioTec.

How to cite: Kullberg, J., Pereira, R., Machadinho, A., and Santos, A.: 4D Digital Twin geological modelling for sustainable quarry management, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17148, https://doi.org/10.5194/egusphere-egu25-17148, 2025.

EGU25-18333 | Posters on site | GI4.2

Utilizing UAVs for Simultaneous DEM Construction and 3D Velocity Tracking in Seepage-Induced Landslide Dam Failures 

Chi-Yao Hung, Yu-Ting Su, Hsin-Yu Wang, and Su-Chin Chen

Advances in UAV technology and data processing platforms have opened new possibilities for studying complex geophysical processes. Landslide dams, formed by large-scale landslides or debris flows, present significant hazards due to their potential for sudden breaching. While overtopping failures have been studied through various scales of experiments, seepage-induced failures remain less understood due to their inherently complex nature. Unlike overtopping, seepage-induced failures are characterized by unpredictable failure locations, internal structural weakening, and dynamic seepage progression, making real-time monitoring particularly difficult. Small-scale laboratory experiments are often inadequate for studying seepage-induced failures due to scaling effects and the inability to fully replicate real-world conditions. This study underscores the importance of conducting large-scale field experiments, where natural seepage processes can be observed in greater detail and under realistic conditions. We introduce an innovative UAV-based framework that employs multiple UAVs equipped with onboard cameras to simultaneously construct high-resolution digital elevation models (DEMs) and track particle motion in 3D to capture the flow field during large-scale seepage-induced dam failure experiments. By coordinating multiple UAVs and applying automated calibration of control points, the system achieves high-precision 3D surface modeling and velocity field extraction in real time. Preliminary results show that this UAV-based approach effectively captures critical seepage-driven structural weakening and internal collapse processes, providing a detailed 3D representation of flow dynamics. The developed methodology addresses key limitations of small-scale laboratory experiments and offers a scalable solution for investigating complex geohazard phenomena. It opens new opportunities for applying UAV technology in geohazard research, including hydrological studies, geomorphological investigations, and disaster mitigation.

How to cite: Hung, C.-Y., Su, Y.-T., Wang, H.-Y., and Chen, S.-C.: Utilizing UAVs for Simultaneous DEM Construction and 3D Velocity Tracking in Seepage-Induced Landslide Dam Failures, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18333, https://doi.org/10.5194/egusphere-egu25-18333, 2025.

EGU25-19518 | Posters on site | GI4.2

Development and application of a multifrequency/multicoil semi airborne UAV-FDEM-system with optimized inductive source 

Arnulf Schiller, Gerhard Kreuzer, Luzian Wolf, and Myeong-Jong Yi

In course of the Project ‘FlowCast’ (ESS Programme / Austrian Academy of Sciences, 2019-2023) a semi-airborne UAV frequency domain EM systems has been developed with the aim of achieving high penetration depths with a UAV sensor system. This required an innovative, powerful inductive source that, due to weight considerations, is designed to be stationary on the ground while the receiver is towed by a drone.  Temporal synchronization of transmitter and receiver takes place via GPS time signal, relative geometry using GPS-RTK recording, correction of the orientation of the receiver using IMU module. In the shallow domain the semi-airborne UAV-EM configuration is compared to a full airborne UAV-EMI system. Both systems can be configured very flexibly in multi-frequency and multi-coil operation and can be optimized for various tasks (conductivity range in the subsurface, penetration depth, resolution). The study presents the hardware development (UAV sensor platform, transmitter, receiver) and data processing (preprocessing and inversion) as well as the results of case studies on test areas around Vienna with buried test bodies or natural structures and ongoing work.

An AIR8 medium lifter (Air6 Systems) octocopter with 25 kg total takeoff mass and 10 kg payload serves as the sensor platform. The receiver is an autonomous sensor system that measures and records amplitude and phase of the magnetic component of a low frequency electromagnetic (EM) signal that is emitted by the stationary transmitter. Auxiliary sensors acquire an accurate time tag, the sensor's GPS position, and the orientation of its main axis. The sensor has a mass of 5 kg, provides sufficient robustness for practical field operations, and can be either hand-positioned along a defined profile, or suspended from an airborne platform that positions the device at a defined position and orientation in 3D space. The combination of position-, amplitude- and phase information of both the receiver and the transmitter allow the estimation of sub-surface electrical conductivity during post-processing of recorded data.

The frequencies to be generated by the transmitter are in the audio range. Wire loop diameter ~ 30m, N=3. A Class D amplifier was developed that voltages up a chopped transmitter signal with a switching frequency of 195 kHz via a transformer and then reassembles it. An FPGA (Field Programmable Logic Array) is used to generate the pulse pattern and the sine signals. This creates a purely digital system. This solution enables large currents in the transmitter loop, thus large dipole moments over a wide frequency range. The 3D inversion program developed at KIGAM is based on the vector finite element method for the 3D electromagnetic forward modeling. The secondary field formulation is used to obtain the secondary field from primary field by ground loop source. 3D resistivity distribution is reconstructed from field EM responses using iterative least squares inversion method adopting active constraint balancing algorithm.

How to cite: Schiller, A., Kreuzer, G., Wolf, L., and Yi, M.-J.: Development and application of a multifrequency/multicoil semi airborne UAV-FDEM-system with optimized inductive source, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19518, https://doi.org/10.5194/egusphere-egu25-19518, 2025.

EGU25-1212 | Orals | GI4.3

Mapping horizontal wind speed using a single Doppler Wind Lidar scanning horizontally: a test case over Paris 

Clement Toupoint, Jonnathan Cespedes, Simone Kotthaus, Ludovic Thobois, Martial Haeffelin, and Janna Preissler

Scanning Doppler Wind Lidars are used in a variety of applications, thanks to the versatility brought by their scanning head. Their principal output is the wind speed along the lidar beam, termed the radial wind speed. When used for vertical profiling, the horizontal wind speed and wind direction are obtained from a wind field reconstruction algorithm (DBS or VAD) applied to the radial wind speed along several high-elevation lines of sight.

However, for other scanning strategies (i.e., with low elevation or horizontal scans), the use of such algorithms is not common, making the radial wind speed the sole output of the Doppler Wind Lidar. The radial wind speed is more difficult to interpret visually for a human user, harder to compare with numerical models, and requires more work to be used into advanced algorithms.

Thus, we showcase the Volume Wind wind field reconstruction algorithm, capable of reconstructing the horizontal wind speed and wind direction from measurement points taken at the same elevation and varying azimuth.

We present data taken from the PANAME2022 campaign, in which a Doppler Wind Lidar (WindCube Scan 400S) was set up on an 88m-high tower in Paris city. The lidar performs scans at 0° elevation above the urban area of Paris, measuring radial wind speed from within the Urban Boundary Layer.  Then, we create maps of horizontal wind speed and direction, spanning a large part of the Paris urban area, using the Volume Wind wind field reconstruction algorithm.

This allows us to study the influence of the topography on the wind field at the height of the urban canopy. The effect of the bed of the Seine river is of particular interest, as it is thought to be an important ventilation corridor in periods of extreme heat. These results highlight the potential of remote sensors for studying the Urban Boundary Layer, and the added value of advanced processing algorithms.

How to cite: Toupoint, C., Cespedes, J., Kotthaus, S., Thobois, L., Haeffelin, M., and Preissler, J.: Mapping horizontal wind speed using a single Doppler Wind Lidar scanning horizontally: a test case over Paris, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1212, https://doi.org/10.5194/egusphere-egu25-1212, 2025.

EGU25-2757 | Orals | GI4.3

Multi product comparison during BELLA-ABL Campaign across different Lidar System 

Donato Summa, Paolo Di Girolamo, Marco Di Paolantonio, Benedetto De Rosa, Ilaria Gandolfi, Giuseppe D'amico, Marco Rosoldi, Michail Mytilinaios, Christina Anna Papanikolaou, Nikolaos Papagiannopoulos, Frabrizio Marra, and Lucia Mona

The BELLA measurement campaign took place at the CNR-IMAA Atmospheric Observatory (CIAO), where a large ensemble of instruments, including ceilometers, a Raman lidar, a wind Doppler lidar, a Ka band Doppler radar, a microwave radiometer and different types of in-situ sensors, were operated on a continuous basis over the period April-June 2024. The measurement effort also benefitted from the continous operation throughout the campaign duration of the Raman lidar system CONCERNIG Lidar, located approx. 7 km south-eastward of CIAO, at University of Basilicata in Potenza. All lidar systems involved in the measurement campaign were operated with high space and time resolution, typically 5-10 m and 10 sec, respectively, with vertical profiling capability both in daytime and nighttime for different atmospheric components/variables, including water vapour mixing ratio, CO2 mixing ratio, temperature and particle (aerosol and clouds) optical (backscatter/extinction) properties. This measurement capability, relying on different ABL tracers/properties is very effective in the characterization of the Atmospheric Boundary Layer structure and depth. Estimates of the ABLH obtained from the different parameters measured by CONCERNING are compared with those obtained from the radiosonde and Raman lidar measurements at CIAO, properly revealing differences associated with the different approaches and with atmospheric variability. In this work our attention is focused on two specific case studies (15-16 April 2024 and 28 April-01 May 2024), with results revealing a good agreement, quantified in terms of absolute and percentage BIAS, between the different sensors and approaches. 

Acknowledgment
The authors acknowledge Next Generation EU Mission 4 “Education and Research” - Component 2: “From research to business” - Investment 3.1: “Fund for the realization of an integrated system of research and innovation infrastructures” - Project IR0000032 – ITINERIS.  

How to cite: Summa, D., Di Girolamo, P., Di Paolantonio, M., De Rosa, B., Gandolfi, I., D'amico, G., Rosoldi, M., Mytilinaios, M., Papanikolaou, C. A., Papagiannopoulos, N., Marra, F., and Mona, L.: Multi product comparison during BELLA-ABL Campaign across different Lidar System, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2757, https://doi.org/10.5194/egusphere-egu25-2757, 2025.

EGU25-2855 | ECS | Orals | GI4.3

3D Wind Field Retrieval within Thunderstorm Clouds over Piedmont 

Priya Kumari, Massimiliano Burlando, Renzo Bechini, Djordje Romanic, and Alessandro Battaglia

Windstorm, particularly driven by thunderstorms, are among the most destructive natural hazards in Europe causing significant economic losses and causalities. Despite various research, the understanding of thunderstorm outflows and their interaction with built and natural environments remains incomplete, especially in regions prone to intense convective activity, such as the northern Italy. This study focuses on the three-dimensional (3D) structure and dynamics of thunderstorm clouds, emphasizing the formation of downburst and gust fronts that generates damaging surface winds. To construct the 3D wind structure, dual Doppler radar systems are utilized, combining data from operational C-band radar and X-Band radar within the study area. A LiDAR instrument was also operational during the investigated event; however, the scanning LiDAR and C-band radar volume do not overlap due to sheltered positioning of the LiDAR relative to the radar. The inclusion of the X-band radar resolves this issue by covering areas that are blind to C-band radar, thereby re-establishing continuity in measurements across the three instruments. This configuration ensures continuous and comprehensive spatial coverage of wind field measurements, spanning from surface to maximum observation altitude.  To carry this out, historical thunderstorm events that occurred in the Piedmont region, Italy, in 2024 are analysed to enhance present understanding of convective dynamics, and the development of severe wind phenomena. This research will also help identify patterns associated with gust fronts and downbursts, hence facilitating improved nowcasting and risk mitigation strategies for these localized windstorms.

How to cite: Kumari, P., Burlando, M., Bechini, R., Romanic, D., and Battaglia, A.: 3D Wind Field Retrieval within Thunderstorm Clouds over Piedmont, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2855, https://doi.org/10.5194/egusphere-egu25-2855, 2025.

EGU25-3198 | ECS | Orals | GI4.3

An airborne Raman lidar to sample horizontal meteorological fields in the framework of MAESTRO 

Hélène Cassan, Patrick Chazette, Julien Totems, Frédéric Laly, Jeremy Lagarrigue, Valentin Guillet, Laurent Forges, and Sandrine Bony

The Airborne Weather and Aerosol Lidar (A-WALI) is the first airborne meteorological lidar using Raman technology to measure the horizontal fields of water vapour, temperature, clouds and aerosols, as key weather and climate parameters (https://metclim-lidars.aeris-data.fr/). Based on lidar technologies tested in WALI (Totems et al., 2021; Chazette et al., 2014)) and ALiAS (Chazette et al., 2020), it was developed to meet the scientific objectives of ERC project MAESTRO (Mesoscale Organisation of Tropical Convection, https://maestro.aeris-data.fr). This experiment was motivated by the scarcity of observations of convective clouds organisation and their environment over the oceans, whereas this spatial organisation of mesoscale clouds, i.e. the tendency of convective clouds to aggregate and form clusters of varying horizontal and vertical extent, plays an important role in climate and meteorology. One of the objectives of the MAESTRO airborne campaign was therefore to sample the horizontal distribution of meteorological temperature and humidity fields, as well as the spatial distribution of aerosols and clouds. A-WALI was flown on board the ATR-42 aircraft of the SAFIRE unit (https://www.safire.fr/), departing from Sal in Cape Verde. The experiment, which took place between 10 August and 10 September 2024, was part of the international campaign ORCESTRA (Organised Convection Experiments in the Tropical Atlantic) supported by the World Climate Research Programme.

We will give examples of the measurements made by A-WALI and estimates of the associated uncertainties. We will discuss the calibration approach, the lidar sampling capabilities and limitations. Depending on the geophysical parameter under consideration, we will show at which spatial scales the lidar measurement provides relevant information and what its range can be.

How to cite: Cassan, H., Chazette, P., Totems, J., Laly, F., Lagarrigue, J., Guillet, V., Forges, L., and Bony, S.: An airborne Raman lidar to sample horizontal meteorological fields in the framework of MAESTRO, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3198, https://doi.org/10.5194/egusphere-egu25-3198, 2025.

In May 2024 the ESA/JAXA satellite mission EarthCARE was launched into a low Earth orbit. The satellite combines a high spectral resolution lidar and a cloud radar with doppler capability as key instruments on one single platform. Additionally, it is equipped with a multi spectral imager and a broad band radiometer. This unique combination makes EarthCARE the most complex single satellite mission to study aerosol, clouds and precipitation. The successful use of these new data for science application needs a thorough validation of the measurements and the derived data products. A similar EarthCARE-like payload was implemented onboard the German research aircraft HALO (High Altitude and Long range).

This instrumentation was flown during PERCUSION (Persistent EarthCARE underflight studies of the ITCZ and organized convection) campaign. Within its scientific component this field experiment aimed to test factors assumed to control the organization of deep maritime convection, and to investigate the influence of convective organization on the larger-scale environment. The validation part of PERCUSION focused on an as close as possible spatial and temporal co-location of the airborne with the space-borne measurement, which can only be done using an aircraft.

Thus, we included an EarthCARE underpass within each research flight. HALO measurements were performed during the EarthCARE commissioning phase in August 2024 out of Sal, Cape Verde, and out of Barbados in September 2024. In addition, we performed pure validation flights out of Oberpfaffenhofen, Germany in November 2024 for the validation under atmospheric conditions that could not be captured in the two first campaign parts. Altogether, 33 EarthCARE underpasses were performed in different aerosol and cloud situations. Some of the flights were coordinated with in-situ measurements onboard other aircraft (e.g. the French ATR42), with shipborne measurements onboard the German research vessel METEOR, or with ground-based radar and lidar measurements at Mindelo (Cape Verde), Barbados, and the ACTRIS stations Antikythera, Leipzig, Lindenberg and Munich.

In our presentation we will give a short overview of the HALO PERCUSION field experiment. Selected EarthCARE underpasses will be used to exemplify the merits and limitations of the level 1 and some level 2 data products of the ATLID lidar onboard EarthCARE.

How to cite: Wirth, M. and Groß, S.: Validation of EarthCARE lidar products using airborne measurements with the research aircraft HALO during the PERCUSION campaign, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3255, https://doi.org/10.5194/egusphere-egu25-3255, 2025.

EGU25-3463 | Orals | GI4.3

Horizontal wind profiling with Doppler lidars: long-term evaluation of the perpendicular vertical sweeps reconstruction method 

Elsa Dieudonné, Pauline Haezebrouck, Perrine Maynard, Anton Sokolov, Hervé Delbarre, Patrick Augustin, and Marc Fourmentin

Over the last 30 years, the demand for wind profile observations in the lower troposphere has rocketed, carried by weather agencies, airports and the wind energy industry. Doppler lidars are favoured for their compactness, easiness of operation, and versatility in the scanning strategy. Several methods have been developed to reconstruct the horizontal wind profile from the raw radial wind observations recorded in different directions. The most common is the Doppler Beam Swinging (DBS) technique, which is implemented in commercial lidars software. However, DBS leaves a blind zone near the ground that can damper the observation of very low-altitude phenomena like certain low-level jets. 
Another horizontal wind reconstruction method consists in combining observations from two vertical sweeps of the Range-Height Indicator (RHI) type recorded in perpendicular directions, by binning the data into horizontal layers. To our knowledge, this cross-RHI technique has only been used twice [1, 2] and applied to only a few tenth  of hours of lidar scans, so that this method still needs to be fully validated over a longer period and under more varied conditions.
In this study, the cross-RHI and DBS techniques were compared using observations recorded by two Doppler scanning lidars from the Leosphere/Vaisala company, installed at two contrasting sites in France: a flat coastal site (Dunkerque, North Sea coast) for four months, and an urban hilly site (Paris) for two months. Compared to the previous studies and to the DBS method, the cross-RHI technique was improved by adding filtering steps designed to remove range-folded echoes from middle-level clouds. In addition, the flow inclination on the hilly site was taken into account by tilting the wind binning layers and minimizing the total intra-layer variance. 
The horizontal wind speed values retrieved using both techniques were in very good agreement on both sites, with correlation coefficients ~0.92 in the first 200 m above the lidar. The regression slope was 0.93 and the intercept was below 0.4 m/s on both sites, drawn by a small share of points where the DBS grossly overestimated the wind speed due to range-folded echoes. This problem disappeared at higher altitudes, where the correlation coefficients exceeded 0.97, with slopes ~0.97 and intercepts lower than 0.1 m/s. In Dunkerque, where the DBS were averaged over 10 consecutive cycles, the horizontal wind direction difference was smaller than 5° (resp. 10°) for 61% (resp. 83%) of observations in the first 200 m above the lidar, and these numbers also improved with increasing altitude. Additionally, the cross-RHI technique proved to be more efficient to reconstruct the wind in pristine conditions yielding low lidar signal. 
This method’s ability to capture very low-altitude phenomena while providing turbulence information opens new perspectives for urban studies and wind farm site assessment. 

References
[1]    R. M. Banta et al., “Nocturnal Low-Level Jet Characteristics Over Kansas During Cases-99,” Bound.-Lay. Meteorol., 105(2), 221–252, 2002, doi: 10.1023/A:1019992330866.
[2]    T. A. Bonin et al., “Evaluation of turbulence measurement techniques from a single Doppler lidar,” Atmos. Meas. Tech., 10(8), 3021–3039, 2017, doi: 10.5194/amt-10-3021-2017.

How to cite: Dieudonné, E., Haezebrouck, P., Maynard, P., Sokolov, A., Delbarre, H., Augustin, P., and Fourmentin, M.: Horizontal wind profiling with Doppler lidars: long-term evaluation of the perpendicular vertical sweeps reconstruction method, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3463, https://doi.org/10.5194/egusphere-egu25-3463, 2025.

EGU25-3558 | ECS | Posters on site | GI4.3

How can the Latent Heat Flux in a Convective Boundary Layer be Described?  

Linus von Klitzing, Diego Lange, David D. Turner, Andreas Behrendt, and Volker Wulfmeyer

We present ongoing work within the Land-Atmosphere Feedback Initiative (LAFI) [1]. LAFI is funded by the Deutsche Forschungsgemeinschaft (DFG) and is located at the University of Hohenheim, Stuttgart. LAFI's objective is to quantify and understand land-atmosphere feedbacks by utilizing synergetic observations and simulations in an interdisciplinary way. One aspect is covered by this work, which aims to provide a better understanding of fluxes in the convective boundary layer (CBL), especially the latent and sensible heat flux. The focus lies on entrainment fluxes in the interfacial layer (IL), the uppermost layer of the CBL, which marks the transition to the free atmosphere (FA).

A key aspect of this work is setting up a comprehensive dataset. This should capture all relevant variables such as temperature, humidity, and wind of the lower atmosphere at high spatial and temporal resolutions for as many cloud-free CBL situations as possible. Accordingly, simultaneous and high-resolution data from the synergetic use of different lidar systems will be used (see [2]) and processed (see [3]). Next, we will analyze this data for the driving variables and possible parameterizations of the latent and sensible heat flux.

We have already started this work by building a dataset containing data from the Atmospheric Radiation Measurement Climate Research Facility (ARM) Southern Great Plains (SGP) site in Oklahoma, USA, and testing a similarity relationship for the latent heat flux in the IL in [4].

Corresponding first results could not confirm the proposed similarity relationship for the latent heat flux in the IL from [2] and will be presented at the conference. Additionally, correlations of the flux with other measured variables, as well as an example case representative for the pool of selected cases will be shown.

In the coming months, we will expand the dataset to other measurement campaigns, like the synergy of Raman and Doppler lidar systems within LAFI in 2025.

References:

[1] https://www.lafi-dfg.de/

[2] Wulfmeyer, Volker et al. (2016): Determination of Convective Boundary Layer Entrainment Fluxes, Dissipation Rates, and the Molecular Destruction of Variances: Theoretical Description and a Strategy for Its Confirmation with a Novel Lidar System Synergy. In Journal of the Atmospheric Sciences 73 (2), pp. 667–692. DOI: 10.1175/JAS-D-14-0392.1

[3] Behrendt, Andreas et al. (2020): Observation of sensible and latent heat flux profiles with lidar. In Atmos. Meas. Tech. 13 (6), pp. 3221–3233. DOI: 10.5194/amt-13-3221-2020

[4] von Klitzing, Linus (2024): Latent Heat Entrainment Flux Similarity Relationships for the Convective Boundary Layer. Master's dissertation. University of Hohenheim, Stuttgart. Institute of Physics and Meteorology

How to cite: von Klitzing, L., Lange, D., Turner, D. D., Behrendt, A., and Wulfmeyer, V.: How can the Latent Heat Flux in a Convective Boundary Layer be Described? , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3558, https://doi.org/10.5194/egusphere-egu25-3558, 2025.

EGU25-4141 | ECS | Orals | GI4.3

Raman lidar derived WVMR profiles compared to ERA5 - A WaLiNeAs application  

Frédéric Laly and Patrick Chazette

Vibrational Raman lidar measurements of the water vapour mixing ratio (WVMR) were conducted during the WaLiNeAs (Water Vapor Lidar Network Assimilation) field campaigns in the western Mediterranean during autumn and winter 2022–2023 and in southwestern France (Toulouse) between June and September 2023. These campaigns, which spanned different seasons and geographical locations, provided an opportunity to sample various meteorological phenomena, including a dry winter, rainstorms, long-range aerosol transport, and an intense heat wave. Consequently, the water vapour content recorded in the lower troposphere showed significant variability during WaLiNeAs, ranging from less than 1 g kg-1 to more than 17 g kg-1. For operational purposes, a vertical resolution of 100 m and a temporal resolution between 15 and 60 min have been chosen. These resolutions are aligned with the spatio-temporal resolution of the ERA5 dataset from ECMWF's Integrated Forecasting System (IFS) global numerical weather prediction models. The processing of the lidar data has resulted in a scientific publication explaining the methods used to invert the lidar data and recover various atmospheric parameters. Lidar measurements address a critical gap left by operational instruments, which struggle to capture the diurnal cycle of water vapour from the planetary boundary layer to the lower free troposphere. The primary aim of this study is to compare ERA5 data with lidar-derived WVMR profiles. The results reveal altitude-dependent differences in Pearson correlation coefficient (COR), mean bias (MB), and root mean square deviation (RMSD), particularly during periods of high-water vapour content (> 10 g kg⁻¹). Over all periods the MB ranges from 0.1 to 3 g kg⁻¹, and the RMSD varies between 0.6 and 3.7 g kg⁻¹. COR ranges from 0.16 to 0.94, with lower values observed in the free troposphere during warmer periods. These variations underline the differences in the performance of the reanalysis model over different periods and altitudes when compared to lidar profiles. We show that the reanalysis constantly underestimated the WVMR at all altitudes. This study highlights the importance of scrutinising WVMR and the challenges faced by models during high water vapour meteorological events. The results provide valuable insights into the performance of operational numerical weather prediction models and highlight the need to refine their representation of WVMR vertical profiles in the lower troposphere by incorporating ground-based lidar measurements.

We give special thanks to the ANR grant #ANR-20-CE04-0001 for its contribution to the WaLiNeAs programme, to Meteo-France for its help with the measurements in Toulouse, and to the CNRS INSU national LEFE programme for its financial contribution to this project.

How to cite: Laly, F. and Chazette, P.: Raman lidar derived WVMR profiles compared to ERA5 - A WaLiNeAs application , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4141, https://doi.org/10.5194/egusphere-egu25-4141, 2025.

EGU25-4413 | ECS | Posters on site | GI4.3

Evaluating Wind Velocity Measurement Errors in Ground-Based Doppler LiDAR Using Virtual Doppler LiDAR and Large Eddy Simulation 

Veronica Escobar-Ruiz, Janet Barlow, and Zheng-Tong Xie

Doppler Wind LiDARs (DWLs) are remote sensing devices that measure wind speed and direction by analysing the Doppler shift of the light backscattered from atmospheric particles along the lidar beam's line of sight. Hence, DWLs are extensively employed in boundary layer meteorology to analyse wind flow due to their ability to provide high-resolution wind measurements. Recently, there has been growing interest in deploying DWLs in urban environments, where mast-based cup anemometers or sonic anemometers face challenges. However, DWL scanning techniques typically assume a homogeneous, stationary wind field, assumptions which often break down in urban boundary layers due to turbulence caused by buildings and complex topography that significantly influences wind profiles. Moreover, the selection of DWL scanning patterns and their configuration should be carefully tailored to the specific application.

One of the most-used scanning methods for measuring vertical wind velocity profiles is the Velocity Azimuth Display (VAD). The technique involves scanning the laser beam around the zenith in a conical pattern at a fixed elevation angle. However, completing the full 360° requires a finite time, during which the wind speed is assumed to be constant. Additionally, if the wind varies significantly within the sampling volume (e.g., due to turbulence or flow inhomogeneity) the calculated wind profiles may be inaccurate.

Large-Eddy Simulation (LES), with a sufficiently high grid resolution to resolve turbulent motions, provides a means to evaluate potential errors in DWL sampling strategies. This study uses a Virtual Doppler LiDAR (VDL) tool (Rahlves et al., 2022) within the Parallelized Large-Eddy Simulation Model (PALM, version 6.0) to estimate velocity profiles derived from simulated radial velocities along virtual laser beam paths under the VAD scheme. The research is part of the ASSURE Project (Across-Scale Processes in Urban Environments), which focuses on Bristol, UK. The project investigates urban wind flow using DWLs deployed across the city, employing scanning strategies utilised during a one-year field campaign beginning in May 2024.

Bristol was chosen for its compact urban layout and distinct topographic features, including the Avon Gorge and a central valley. The city serves as a case study for examining urban wind dynamics. This study's objectives are twofold: (1) to identify and quantify errors between the vertical wind profile derived from a VAD scan using the VDL and the profile directly taken from the PALM model and (2) to facilitate comparisons between PALM-simulated wind profiles and observations from ground-based DWL. By addressing the discrepancies arising from topographically induced flow, this research aims to enhance the reliability of DWL data in urban settings and improve our understanding of urban boundary layer processes. Results will be presented for a case study of flow channelled by a deep valley interacting with a city-centre boundary layer.

Rahlves, C., Beyrich, F., and Raasch, S. (2022). ‘‘Scan strategies for wind profiling with Doppler lidar – an large-eddy simulation (LES)-based evaluation’’, Atmospheric Measurement Techniques, 15(9), 2839-2856

How to cite: Escobar-Ruiz, V., Barlow, J., and Xie, Z.-T.: Evaluating Wind Velocity Measurement Errors in Ground-Based Doppler LiDAR Using Virtual Doppler LiDAR and Large Eddy Simulation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4413, https://doi.org/10.5194/egusphere-egu25-4413, 2025.

Atmospheric lidar has become a powerful tool for atmospheric detection due to its advantages of high spatiotemporal resolution, multiple parameters and high-precision detection. In this paper, the application status of lidar in China’s meteorological observation is introduced, and the prospects for the development of lidar applications are presented. For better observation of atmospheric clouds, aerosol, and water vapor parameters, the China Meteorological Administration(CMA) has laid out and constructed a Raman-Mie aerosol lidar network with 49 stations from 2021 to 2024 and has solved several key technical problems such as data quality control, parameter inversion, and quantitative calibration. In order to achieve high-precision observations with a time resolution at the minute level, more than 10 standard specifications have been formulated for calibration, observation, and data transmission. The lidars for network applications normally use a three-wavelength laser covering 355 nm, 532 nm, and 1064 nm,and they can achieve a detection distance of more than 10 km, an accuracy of aerosol backscattering coefficient of less than 20%(0.5-2 km)and 40%(2-5 km), and an accuracy of water vapor concentration of less than 1g/kg (0.5-3 km).In the field of wind observation, the CMA has laid out and constructed a wind lidar network with 372 stations by 2024. The lidars use the coherent detection with a laser wavelenth of 1550nm, and they can achieve a maximum detection distance of more than 3km, a horizontal wind speed error less than 0.8m/s, and a horizontal wind direction error less than 8°.The layout and application of aerosol lidar network and wind lidar network have greatly improved China's meteorological observation capability and application levels in aerosol and wind fields. In recent years, the CMA has actively cooperated with various universities and scientific research institutes to carry out key technological studies in atmospheric temperature and humidity lidar, high spectral resolution lidar, middle and upper atmosphere lidar, and airborne/spaceborne lidar. Through planning and constructing meteorological business application platforms in the future, the comprehensive three-dimensional observation of multiple parameters such as temperature, humidity, wind and aerosols will be developed to improve China's meteorological observation ability and provide strong support for research in meteorological services, atmospheric science and climate change.

How to cite: Chen, Y.: Status and Development of Lidar applications in China's Meteorological Observation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5725, https://doi.org/10.5194/egusphere-egu25-5725, 2025.

EGU25-5758 | Orals | GI4.3

Aerosol impacts on cirrus cloud formation and properties using in-situ and lidar measurements during CIRRUS-HL campaign  

Qiang Li, Silke Gross, Martin Wirth, Tina Jurkat-Witschas, Christiane Voigt, Elena De La Torre Castro, and Daniel Sauer

Cirrus clouds cover about 30% of the Earth’s surface and play a crucial role in the Earth’s radiation balance. They are composed of ice crystals with various sizes and nonspherical shapes. Ice crystals can form through either homogeneous freezing or heterogeneous freezing depending on the ambient temperature, humidity, updraft, and the availability of INPs, and hence possess different properties. Their radiative effects strongly depend on the formation processes and cloud microphysical, thermal, and optical properties. Furthermore, global aviation affects the Earth’s radiation balance by increasing cloudiness due to contrail formation and exerting an indirect effect on the microphysical properties of naturally-formed cirrus clouds. Aviation is responsible for 3-4% of anthropogenic effective radiative forcing and more than half of them stems from contrails and contrail-induced cirrus. Experimental and numerical studies have been carried out in the past years to understand contrails and contrail-induced cirrus as well as their climate effects. Unfortunately, however, the parameterization of ice crystal properties in global climate model and the estimate of radiation forcings are still inadequate. Compared with the intensive studies on cirrus clouds in the tropics and midlatitude regions, cirrus cloud measurements and model studies at high latitudes are sparse, although cirrus clouds at high latitudes attract more attention in recent years because the Arctic undergoes faster warming than other regions of the globe. The airborne measurements from the ML-CIRRUS mission revealed that cirrus clouds with enhanced PLDR appear in areas of high aviation emissions. Nevertheless, observational evidence of indirect effects of aviation exhaust on the changes of cirrus properties is still missing. Thanks to the foundational work of ML-CIRRUS, the CIRRUS-HL mission in June-July, 2021, with upgraded instrumentation was designed to characterize cirrus cloud at both high- and midlatitudes and to investigate aviation impact, radiation, and aerosol-cloud interactions. It collected more details in the simultaneous profiling of cirrus cloud and aerosol properties. In this study, we focus on the comparison of particle linear depolarization ratios (PLDR) of cirrus clouds with the airborne lidar WALES from two specific flights under similar cloud formation processes during CIRRUS-HL. Their microphysical properties (i.e. ice crystal size and number concentration) are also determined and compared based on the analysis of simultaneous in-situ measurements. The analysis is also extended to all the flights for statistical results. Furthermore, the characterization of aerosol load, especially aviation soot, will be identified in the regions of ice crystal formation and evolution and their correlations with cirrus cloud properties are finally able to be further determined.  

How to cite: Li, Q., Gross, S., Wirth, M., Jurkat-Witschas, T., Voigt, C., De La Torre Castro, E., and Sauer, D.: Aerosol impacts on cirrus cloud formation and properties using in-situ and lidar measurements during CIRRUS-HL campaign , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5758, https://doi.org/10.5194/egusphere-egu25-5758, 2025.

EGU25-6889 | Orals | GI4.3

Desert dust profiling and applications 

Vassilis Amiridis

Atmospheric remote sensing from space and surface has been advanced during the last decade. Mineral dust is an atmospheric target that provides a strong signature on active and passive polarimetric remote sensing observations, due to its irregular shape. Nowadays, advanced lidar systems operating in the framework of ACTRIS provide quality assured, calibrated multi-wavelength linear particle depolarization ratio measurements, while new developments will provide us elliptical polarization recordings in the near future. Passive polarimeters are already part of ACTRIS and AERONET and their integration in operational algorithms is expected in the near future. This wealth of new information combined with updated scattering databases and sophisticated inversion schemes provide the means towards an improved characterization of desert dust in the future. This kind of information can be used for space-borne lidars such as CALIPSO, CATS, Aeolus, EarthCARE and the future AOS missions.

We present here some examples of how remote sensing facilitates desert dust research during the last decade, aiming to demonstrate the progress on issues such as: (a) the discrimination of desert dust in external mixtures, (b) the estimation of the fine and coarse particle modes, (c) the synergy of passive and active remote sensing for the derivation of dust properties, (d) the provision of dust-related CCN and IN particle concentrations for aerosol-cloud interaction studies, (e) the development of new scattering databases based on realistic particle shapes, (e) the application of these techniques on space lidar datasets for the provision of climatological datasets, and (f) the use of these datasets in data assimilation for improving dust representations in models.

How to cite: Amiridis, V.: Desert dust profiling and applications, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6889, https://doi.org/10.5194/egusphere-egu25-6889, 2025.

EGU25-7172 | Posters on site | GI4.3

Recent Advances in Automated Temperature and Humidity Lidar 

Andreas Behrendt, Diego Lange, and Volker Wulfmeyer

We will give an update of our recent activities regarding automated high-resolution temperature and humidity lidar.

The Raman lidar ARTHUS (Atmospheric Raman Temperature and HUmidity Sounder) of University of Hohenheim is an automated instrument with continuous operation (Lange et al., 2019; Wulfmeyer and Behrendt, 2022). Besides being operated during several field campaigns elsewhere, ARTHUS is usually located at the LAFO (Land Atmospheric Feedback Observatory) near the agricultural research fields of our university. Here, in addition, three scanning Doppler lidars, a Doppler cloud radar, two meteorological 10-m towers with eddy-covariance stations, as well as surface and sub-surface sensors are collecting routinely data. These data are combined with detailed vegetation analyses.

ARTHUS is an eyesafe Raman lidar using a diode-pumped Nd:YAG laser as transmitter. Only the third-harmonic radiation at 355 nm is – after beam expansion – transmitted into the atmosphere. The laser power is about 20 W at 200 Hz repetition rate. The receiving telescope has a diameter of 40 cm. A polychromator extracts the elastic backscatter signal and four inelastic signals, namely the vibrational Raman signal of water vapor and CO2 molecules, and two pure rotational Raman signals. The raw data is stored with a resolution of 7.5 m and typically 1 to 10 s. All five signals are simultaneously analyzed and stored in both photon-counting (PC) mode and voltage (so-called “analog” mode) in order to make optimum use of the large intensity range of the backscatter signals covering several orders of magnitude. Primary data products are temperature, water vapor mixing ratio, carbon dioxide mixing ratio, particle backscatter coefficient, and particle extinction coefficient. The high resolution allows studies of boundary layer turbulence (Behrendt et al, 2015) and - in combination with the vertical pointing Doppler lidar - sensible and latent heat fluxes (Behrendt et al, 2020).

Further refined lidars like ARTHUS are offered by the company Purple Pulse Lidar Systems (www.purplepulselidar.com). Meanwhile three more systems have been built and are operating.

At the conference, we will present the recent advances in these powerful automated temperature and humidity lidars and show highlights of the measurements.

 

References:

Behrendt et al. 2015, https://doi.org/10.5194/acp-15-5485-2015

Behrendt et al. 2020, https://doi.org/10.5194/amt-13-3221-2020

Lange et al. 2019, https://doi.org/10.1029/2019GL085774

Wulfmeyer and Behrendt 2022, https://doi.org/10.1007/978-3-030-52171-4_25

How to cite: Behrendt, A., Lange, D., and Wulfmeyer, V.: Recent Advances in Automated Temperature and Humidity Lidar, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7172, https://doi.org/10.5194/egusphere-egu25-7172, 2025.

EGU25-7552 | Posters on site | GI4.3

Scanning Measurements With an Automated Temperature and Moisture Lidar in the Atmospheric Boundary Layer 

Diego Lange Vega, Andreas Behrendt, and Volker Wulfmeyer

Despite significant advancements in atmospheric observation techniques, the thermodynamic structure of the atmospheric boundary layer (ABL) remains largely unexplored due to the scarcity of suitable high-resolution remote sensing measurements. Over the past six years, the Atmospheric Raman Temperature and Humidity Sounder (ARTHUS), an automated profiler based on the Raman lidar technique (Lange et al., 2019), has participated in several ground- and ship-based measurement campaigns (Stevens et al., 2021; Flamant et al., 2021). These campaigns have demonstrated ARTHUS's capability to resolve critical atmospheric features, such as turbulent fluctuations and their statistics with high temporal and spatial resolution.

In combination with Doppler lidars, ARTHUS enables profiling of sensible and latent heat fluxes within the convective ABL, thereby supporting the investigation of flux-gradient relationships (Wulfmeyer et al. 2016, Behrendt et al., 2020). These capabilities make ARTHUS a powerful tool for advancing process studies of land-atmosphere interactions, enhancing weather and climate monitoring, validating atmospheric models, and improving data assimilation techniques. We present examples from several field campaigns with respect to the observation of diurnal cycles of profiles of mean and turbulent variables.

An eye-safe Nd:YAG laser with 20 W at 355-nm is used as transmitter. A 40-cm receiving telescope collects backscattered light providing independent measurements of temperature (T), water vapor mixing ratio (WVMR), CO2 concentration, particle extinction coefficient, and particle backscatter coefficient.

ARTHUS has proven its reliability during extended operations at the Land Atmosphere Feedback Observatory (LAFO) at the University of Hohenheim and across various field campaigns under diverse atmospheric conditions. As part of the Land-Atmosphere Feedback Initiative (LAFI, Wulfmeyer et al. 2024), ARTHUS will extend its capabilities to include scanning measurements from the surface through the ABL, capturing three-dimensional turbulent structures with a focus on entrainment processes. The campaign will take place between March and August 2025 at the LAFO site. For the first time, ARTHUS will deliver comprehensive maps of T, WVMR, and CO₂, especially near the surface and canopy but also up to the top of the ABL offering unprecedented insights into land-atmosphere feedback. At the conference, highlights of the first LAFI measurements will be shown.

References:

Lange et al. 2019, https://doi.org/10.1029/2019GL085774

Stevens et. al. 2021, https://doi.org/10.5194/essd-2021-18

Flamant et al. 2021, https://doi.org/10.1007/s42865-021-00037-6

Behrendt et al. 2020, https://doi.org/10.5194/amt-13-3221-2020

Wulfmeyer et al. 2016, https://doi.org/10.1175/JAS-D-14-0392.1

Wulfmeyer et al. 2024, https://doi.org/10.5194/egusphere-egu24-10102

How to cite: Lange Vega, D., Behrendt, A., and Wulfmeyer, V.: Scanning Measurements With an Automated Temperature and Moisture Lidar in the Atmospheric Boundary Layer, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7552, https://doi.org/10.5194/egusphere-egu25-7552, 2025.

EGU25-8390 | Orals | GI4.3

New operational perspective to identify aerosol in real-time with a pioneering algorithm (CONIOPOL) based on CL61 data 

Quentin Laffineur, Alexander Mangold, Karen De Causmaecker, and Andy Delcloo

In recent years, there has been an increase in the intensity and frequency of smoke plume events over North America (sometimes reaching Europe) and dust plume events reaching Europe from Africa. As these can potentially affect surface air quality, environmental agencies are increasingly interested in being able to identify the nature of aerosol plumes, monitor it in real time and determine whether its interaction with the atmospheric boundary layer will impact surface air quality. The automatic LIDAR-ceilometer (ALC) primarily designed for cloud base height detection has greatly improved over the last years and now provides vertical profiles of backscatter from aerosols and clouds. Recently, a new type of ALC with a depolarization function (VAISALA CL61) is commercially available for distinguishing cloud phase (which is useful for weather forecasting) and also makes it possible to support the type identification of aerosols.

At the Royal Meteorological Institute of Belgium (RMI), we have been developing a new pioneering algorithm (CONIOPOL: CONIOlogy + POLarization) based only on CL61 measurements (backscatter and depolarization profiles) to provide in real-time automatic identification of cloud phase, precipitation type and aerosol type. CONIOPOL cannot provide an independent and unambiguous identification of the aerosol type because the CL61 operates with a single wavelength. Although, CONIOPOL is a very useful operational support allowing a quick identification in real time of the type of aerosols in combination with forecasts and backward trajectories models.

The effectiveness and robustness of CONIOPOL will be demonstrated in different ways, through case studies comparing its output with CAMS forecast and air quality measurements, through statistical analysis of CONIOPOL output and by a comparison analysis between CONIOPOL output and CAMS forecasts. In addition to its operational use, it is capable of assembling a climatology of cloud phase, precipitation type and aerosol type. Further, it can contribute to the validation of EarthCARE (ESA) space-borne products.

How to cite: Laffineur, Q., Mangold, A., De Causmaecker, K., and Delcloo, A.: New operational perspective to identify aerosol in real-time with a pioneering algorithm (CONIOPOL) based on CL61 data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8390, https://doi.org/10.5194/egusphere-egu25-8390, 2025.

EGU25-8397 | Posters on site | GI4.3

A Study Mass Extinction Efficiency (MEE) Calculation and Variability Analysis by Aerosol Source Identification: Application of Horizontal Scanning Lidar and HYSPLIT Model 

Jihyun Yoon, Juseon Shin, Sohee Joo, Gahyeon Park, Dukhyeon Kim, and Youngmin Noh

South Korea faces complex air quality challenges arising from domestic emission sources driven by industrialization and urbanization, as well as seasonally influenced long-range transport pollutants from overseas. In particular, springtime dust storms and wintertime heating emissions both domestic and foreign converge to create a multifaceted air pollution environment. To effectively understand and manage these issues, accurately determining the Mass Extinction Efficiency (MEE) based on optical observations is essential. In this study, we refined MEE calculations by integrating LiDAR-based observations with ground-level measurements, analyzed variability as a function of aerosol origin, and simultaneously assessed the potential for indirect evaluation of atmospheric composition. Using a horizontal SCANNING LiDAR, we derived high-resolution, two-dimensional extinction coefficients near the surface and combined these data with hourly Particulate Matter (PM) observations from the AirKorea monitoring network. Employing the Ångström exponent to differentiate coarse mode particles (Ångström exponent ≈ 0) from fine mode particles (Ångström exponent ≈ 3), we calculated extinction coefficients for total, coarse, and fine aerosols. We then derived MEE values through three approaches: total extinction coefficient relative to PM10, coarse extinction coefficient relative to (PM10 – PM2.5), and fine extinction coefficient relative to PM2.5. To analyze aerosol origins, we used the HYSPLIT (Hybrid Single-Particle Lagrangian Integrated Trajectory) model of NOAA(National Oceanic and Atmospheric Administration), which allowed us to evaluate mesoscale and regional source contributions and investigate their impact on MEE variability. Data from December 2021 to the present revealed substantial variations in MEE values depending on aerosol source regions and compositions. By offering a refined analytical framework tailored to South Korea’s unique climatic and geographical characteristics, this study provides valuable insights for improved air quality monitoring and predictive modeling.

"This research was supported by Particulate Matter Management Specialized Graduate Program through the Korea Environmental Industry & Technology Institute(KEITI) funded by the Ministry of Environment(MOE)"

How to cite: Yoon, J., Shin, J., Joo, S., Park, G., Kim, D., and Noh, Y.: A Study Mass Extinction Efficiency (MEE) Calculation and Variability Analysis by Aerosol Source Identification: Application of Horizontal Scanning Lidar and HYSPLIT Model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8397, https://doi.org/10.5194/egusphere-egu25-8397, 2025.

EGU25-8530 | Orals | GI4.3

 Improvement of DQ-1/ACDL in Global Thin Cirrus Cloud Detection 

Sijie Chen, Bo Li, and Kai Zhang

Lidar is an essential and unique tool in the current integrated spaceborne remote sensing observation system. From CALIPSO-CloudSat in the A-Train constellation to China’s Daqi-1 (DQ-1) and the latest EarthCARE mission, lidar’s ability to detect thin cirrus and low clouds with fine vertical resolution has significant implications. The effective combination of lidar and CPR provides a complete cloud vertical structure for related studies and an accurate validation for passive remote sensors.

Launched successfully on April 16, 2022, the DQ-1 satellite carries the Aerosol Carbon Detection Lidar (ACDL), a three-wavelength  (532, 1064, and 1572 nm) lidar for comprehensive measurements of atmosphere composition. is technically a combination of two lidars with different mechanisms: a high-spectral-resolution lidar (HSRL) measuring clouds and aerosols and an integrated-path differential absorption (IPDA) lidar measuring carbon dioxide. The mechanism of HSRL allows the separation of aerosol contribution from the molecular backscatter, therefore removing the lidar ratio assumption in the traditional Mie-scattering lidar like CALIOP. Initial validation results indicate an accuracy better than 20% for a strong signal backscatter profile with 24 m vertical resolution. The cloud-top and base height, phase, and classification products have been processed accordingly.

Positioned time-wise between CALIPSO and EarthCARE missions, DQ-1 fills a critical gap in the observation and cross-validation. This report contains results from a one-year-long comparison between DQ-1/ACDL and CALIPSO/CALIOP from June 2022 to June 2023, till the end of CALIPSO operation. The analysis includes case studies from different latitudes and scenarios, and overall gridded global thin cirrus cloud distributions. The results show good consistency between the two systems, with DQ-1/ACDL demonstrating better coherence and performance. Depending on data availability, the report might also include preliminary comparisons with EarthCARE/ATLID data. The report will highlight key improvements of the DQ-1/ACDL system in thin cirrus cloud detection, for better monitoring and valuable insights of cloud properties, atmospheric dynamics, and climate modeling.

How to cite: Chen, S., Li, B., and Zhang, K.:  Improvement of DQ-1/ACDL in Global Thin Cirrus Cloud Detection, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8530, https://doi.org/10.5194/egusphere-egu25-8530, 2025.

The Cloud and Aerosol Lidar for Global Scale Observations of the Ocean-Land-Atmosphere System (CALIGOLA) is an advanced multi-purpose space lidar mission with a focus on atmospheric and oceanic observation aimed at characterizing the Ocean-Earth-Atmosphere system and the mutual interactions within it. This mission has been conceived by the Italian Space Agency (ASI) with the aim to provide the international scientific community with an unprecedented dataset of geophysical parameters capable of increasing scientific knowledge in the areas of atmospheric, aquatic, terrestrial, cryospheric and hydrological sciences. The Italian Space Agency is partnering with NASA on this exciting new space lidar mission. The mission is planned to be launched in the time frame 2031-2032, with an expected lifetime of 3-5.

Exploiting the three Nd:YAG laser emissions at 354.7, 532 and 1064 nm and the elastic (Rayleigh-Mie), depolarized, Raman and fluorescent lidar echoes from atmospheric and ocean constituents, CALIGOLA will carry out multi-wavelength profile measurements of the backscatter, extinction and fluorescent coefficient and the depolarization ratio of atmospheric and ocean particles. These measurements will enable determinations of the microphysical and dimensional properties of atmospheric aerosols and clouds and their typing. Measurements of ocean optical properties will document phytoplankton seasonal and inter-annual dynamics and will improve understanding on marine biogeochemistry, the global carbon cycle, and responses of plankton ecosystems to climate variability. One specific measurement channel at 685 nm will be dedicated to fluorescence measurements from atmospheric aerosols and marine chlorophyll, for the purpose of aerosol typing and characterization of phytoplankton nutrient stress and primary production. CALIGOLA will provide accurate measurements of small-scale variability in earth surface elevation, primarily associated with variations in the ice and snow, terrain, and terrestrial vegetation height (e.g., forest canopies).

Phase A studies, commissioned by the Italian Space Agency to Leonardo S.p.A. and focusing of the technological feasibility of the laser source and the receiver, were conducted from October 2022, while Phase A/B1 activities for the payload, platform, and end-to-end system will start in January-February 2025. Scientific studies in support of the mission are ongoing, commissioned by the Italian Space Agency to University of Basilicata (KO: November 2021) and ISMAR-CNR (KO: September 2023). In September 2023, NASA-LARC initiated a pre-formulation study to assess the feasibility of a possible contribution to the CALIGOLA mission focused on development of the detection system and sampling chain and the implementation of data down link capabilities. The pre-formulation study ended in September 2024, the Mission Concept Review was successfully completed, and a phase A/formulation study has been finalized in preparation for a System Requirements Review, which should start shortly. This presentation will provide details on current status and future steps of this groundbreaking multidisciplinary lidar mission.

How to cite: Di Girolamo, P. and the CALIGOLA Team: The Cloud and Aerosol Lidar for Global Scale Observations (CALIGOLA): Overview of the current status and future steps of a groundbreaking multidisciplinary Mission, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8567, https://doi.org/10.5194/egusphere-egu25-8567, 2025.

EGU25-8872 | ECS | Posters on site | GI4.3

CO2 Measurements with Raman Lidar in the Lower Troposphere  

Moritz Schumacher, Diego Lange, Andreas Behrendt, and Volker Wulfmeyer

Carbon dioxide is the most important greenhouse gas caused by emissions from human activities. Nevertheless, little is known about its distribution in the atmposphere. Thus, continuous CO2 measurements not only on the ground but also in higher altitudes are key to improve our understanding of radiative forcing. Therefore, ground-based lidar systems with their ability of range-resolved CO2 measurements are particularly interesting. In the recent two years, we have developed and incorporated a new channel to our ground-based Raman lidar system ARTHUS ("Atmospheric Raman Temperature and HUmidity Sounder") [1] and successfully collected more then 70 days of CO2 profiles at the “Land-Atmosphere Feedback Observatory” (LAFO), in Stuttgart, Germany [2]. We utilize the 2ν2 CO2 Raman line, which is well separated from Raman lines of other atmosphere gases, especially O2. With the current setup, we profile CO2, temperature and humidity as well as particle extinction and particle backscatter coefficients in five receiver channels. The first CO2measurements in 2023 with a preliminary calibration where already presented at the EGU24 [3]. Since then, the laser power has been doubled while still being an eye-safe system. With some other improvements in addition, the integration times needed at night and for a resolution of 300 m are for example 1.5 hours for an uncertainty of 1.5 ppm and 2 hours for an uncertainty of 2 ppm at altitudes of 500 m and 1 km, respectively.

We are currently (January 2025) adding a 2-mirror scanner to the system. With this, we will much better calibrate our CO2 mixing ratio with low-level scans near our ground-based in-situ sensors located at the LAFO site. The scanning measuements of the CO2 concentration will provide insights in its distribution around the surface sensors and enable us to identify and quantify local carbon sources and sinks. We will present the recent approaches and first scanning measurements at the EGU25.

References: 

[1] Lange, D. et al.: Compact Operational Tropospheric Water Vapor and Temperature Raman Lidar with Turbulence Resolution. Geophys. Res. Lett. (2019). DOI: 10.1029/2019GL085774 

[2] Späth, F., S. Morandage, A. Behrendt, T. Streck, and V. Wulfmeyer, 2021: The Land-Atmosphere Feedback Observatory (LAFO). EGU21-7693 (2021). DOI: 10.5194/egusphere-egu21-7693 

[3] Schumacher, M., D. Lange, A. Behrendt, V. Wulfmeyer, 2024: Measurements of CO2Profiles in the Lower Troposphere with the new Raman Lidar Channel of ARTHUS. EGU24-9219 (2024). DOI: 10.5194/egusphere-egu24-9219 

How to cite: Schumacher, M., Lange, D., Behrendt, A., and Wulfmeyer, V.: CO2 Measurements with Raman Lidar in the Lower Troposphere , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8872, https://doi.org/10.5194/egusphere-egu25-8872, 2025.

EGU25-9052 | ECS | Posters on site | GI4.3

Evaluating the MONARCH Model with Lidar Data: A Step Toward Improving Global Dust Surface Concentrations 

Carlotta Gilè, Emanuele Emili, Jeronimo Escribano, Luka Ilic, Oriol Jorba Casellas, and Carlos Perez Garcia Pando

The Barcelona Dust Regional Center (BDRC) provides daily forecasts of dust optical depth and dust surface concentrations, as part and coordination entity of the Northern Africa, Middle East and Europe (NAMEE) node of the World Meteorological Organization Sand and Dust Storm Warning Advisory and Assessment System (WMO SDS-WAS). Dust optical depth forecasts from the NAMEE SDS-WAS ensemble show a relatively good agreement, while the forecasts of dust surface concentrations show larger variability between models. Moreover, the consistency between dust optical depth, as an integrated column quantity, and surface concentration forecasts remains challenging. 

Since July 2024, vertical profiles of dust concentrations from the Multiscale Online Nonhydrostatic AtmospheRe Chemistry (MONARCH) model of the SDS-WAS ensemble have been made public on the BDRC website. This study presents the first evaluation of this new forecast product through comparisons with lidar observations, focusing on vertical profiles of total and dust extinction coefficients. Specifically, we used lidar measurements from the NASA Micro-Pulse Lidar Network (MPLNET) in the Mediterranean and North Africa area. While the comparison of the total extinction coefficient between MONARCH (550 nm) and MPLNET (532 nm) can be performed directly but is affected by unaccounted aerosols (e.g. sea salts, anthropogenic aerosols), the extraction of dust extinction coefficient from MPLNET products required additional processing. To this purpose, the POLIPHON algorithm was exploited to obtain the lidar-derived dust component from the total aerosol load and enable a fair intercomparison with modeled dust profiles. Initial descriptive and quantitative results confirm the model’s reliability in forecasting and predicting dust vertical profile characteristics.

Building on this evaluation, we explore the potential of leveraging lidar data to improve the dust ground concentration estimates of the MONARCH model forecasts. The proposed approach explores empirical adjustments of the model's surface concentration using lidar observations and validates these improvements against independent ground-based PM10 measurements collected by the European Environment Agency (EEA). The analysis is performed for three European sites, namely Tenerife, Barcelona, and El Arenosillo, for the period from July 2024 to January 2025.

The expanded aim of this work is to assess the feasibility of utilizing next-generation space-borne lidar systems, such as EarthCARE (Cloud, Aerosol, and Radiation Explorer), to enhance global dust surface concentration estimations from model forecasts.

This study highlights the synergy between observations and modeling, demonstrating how lidar observations could be exploited for correcting and improving model performance at both regional and global scales.

How to cite: Gilè, C., Emili, E., Escribano, J., Ilic, L., Jorba Casellas, O., and Perez Garcia Pando, C.: Evaluating the MONARCH Model with Lidar Data: A Step Toward Improving Global Dust Surface Concentrations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9052, https://doi.org/10.5194/egusphere-egu25-9052, 2025.

EGU25-10120 | ECS | Orals | GI4.3

Comparison of fresh and aged smoke particles simultaneously observed at the ACTRIS Potenza observatory  

Benedetto De Rosa, Nikolaos Papagiannopoulos, Michail Mytilinaios, Aldo Amodeo, Giuseppe D'Amico, Marco Rosoldi, Donato Summa, Ilaria Gandolfi, Christina–Anna Papanikolaou, Pilar Gumà-Claramunt, Teresa Laurita, Francesco Cardellicchio, Igor Veselovskii, Paolo Di Girolamo, and Lucia Mona

This study presents a detailed analysis of the optical and microphysical properties of biomass burning aerosols from two distinct smoke plumes observed on 16 July 2024 at the CIAO atmospheric observatory in Potenza, Italy. The lower layer corresponds to a local wildfire, while the upper layer correspond to  a long-range transported plume from Canada. The objective is to highlight significant differences in their characteristics and atmospheric impacts.

The local fire was characterized not only with lidar measurements, but with all the remote sensing instruments present in the observatory. The fire, ignited around 16:00 UTC approximately 2 km from the observatory, was detected within an hour. Ceilometer lidar and radar data showed that wildfire particles ascended to 3 km, where elevated humidity facilitated the formation of condensation nuclei, confirmed by a radiometer-observed peak in liquid water content. The ACSM (Aerosol Chemical Speciation Monitor) and aethalometer measurements show a significant peak around 20:00 UTC, which coincides with the deposition of the particles. The inversion results from lidar measurements revealed a low contribution of black carbon and fine-mode particles, consistent with incomplete combustion typical of small-scale fires. Furthermore, a strong dependence on humidity variations was observed, emphasizing the dynamic interaction between local fires and atmospheric conditions.

In contrast, the Canadian wildfire plume, transported at altitudes between 5.5 and 6.5 km, exhibited different characteristics. Due the complete combustion particles have a higher absorption properties. The lidar ratio at 532 nm exceeded that at 355 nm, similar with previous observations of aged wildfire plumes. During long-range transport, aging processes such as coagulation significantly altered the particles, increasing their effective radius. Microphysical analysis indicated the presence of larger, more absorbent particles compared to the local plume.

This study underscores the importance of integrating remote sensing and in-situ measurements to capture the lifecycle of wildfire events. The results reveal a great variability in smoke plume properties, which must be accounted for in radiative transfer models to accurately assess their atmospheric and climatic impacts.

How to cite: De Rosa, B., Papagiannopoulos, N., Mytilinaios, M., Amodeo, A., D'Amico, G., Rosoldi, M., Summa, D., Gandolfi, I., Papanikolaou, C., Gumà-Claramunt, P., Laurita, T., Cardellicchio, F., Veselovskii, I., Di Girolamo, P., and Mona, L.: Comparison of fresh and aged smoke particles simultaneously observed at the ACTRIS Potenza observatory , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10120, https://doi.org/10.5194/egusphere-egu25-10120, 2025.

EGU25-10454 | ECS | Orals | GI4.3

Raman lidar water vapor observations to assess the uncertainty of MLS and ERA5 at the upper troposhere 

Dunya Alraddawi, Philippe Keckhut, Florian Mandija, Guillaume Payen, Jean Charles Dupont, Christophe Pietras, Abdenour Irbah, Alain Sarkissian, Alain Hauchecorne, and Jacques Porteneuve

Water vapor information in the upper troposphere (UT) is crucial for understanding the thermodynamic conditions leading to the formation of cirrus clouds and persistent contrails. Both phenomena significantly contribute to aviation-induced radiative forcing, driving global mitigation efforts. Raman lidars provide high-resolution humidity profiles, describing altitudes prone to ice supersaturation—conditions that are challenging to detect and accurately represent in current models.

In this study, Raman lidar Water Vapor Mixing Ratio (WVMR) measurements from various sites in France were used to evaluate the performance of the ERA5 model in assessing humidity at typical aircraft altitudes. Additionally, the uncertainties in Microwave Limb Sounder (MLS) WVMR measurements at the same altitudes were assessed. Raman lidar profiles were aggregated into pseudo-monthly datasets to facilitate comparison with the limited number of MLS overpasses at each site, enabling validation of spatio-temporal pseudo-monthly lidar-matched MLS and ERA5 WVMR profiles.

The MLS dataset offers one of the longest records of WVMR, making it a valuable resource for trend assessment. This investigation enables the validated use of these datasets for studying UT humidity trends and variability on seasonal and annual scales over the past decade.

How to cite: Alraddawi, D., Keckhut, P., Mandija, F., Payen, G., Dupont, J. C., Pietras, C., Irbah, A., Sarkissian, A., Hauchecorne, A., and Porteneuve, J.: Raman lidar water vapor observations to assess the uncertainty of MLS and ERA5 at the upper troposhere, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10454, https://doi.org/10.5194/egusphere-egu25-10454, 2025.

EGU25-10784 | Posters on site | GI4.3

Real-Time Monitoring of Air Pollution and Detection of Illegal Emissions Using Advanced Scanning LiDAR Technology 

Seong-min Kim, Kwanchul Kim, Gahye Lee, Jeong-min Park, Sea-ho Oh, Min-kyung Sung, Sangcheol Kim, Youndae Jung, Ilkwon Yang, Byung-Jin Choi, Sungchul Choi, and Changgi Choi

Air pollution is a persistent environmental and public health challenge, particularly in industrial areas characterized by diverse and diffuse emission sources. This study demonstrates the application of an advanced scanning LiDAR system for real-time monitoring of particulate matter (PM2.5, PM10) and the detection of illegal emissions in Gyeonggi Province, South Korea. The system employs advanced remote sensing technology, enabling 360° atmospheric scans within a 5 km radius at 30-minute intervals, with a spatial resolution of 30 meters.

During its deployment in the Sihwa National Industrial Complex, home to over 978 industrial facilities, the LiDAR system identified 192 potential illegal emission sources. Subsequent investigations confirmed 22 violations of environmental regulations, resulting in regulatory actions such as facility shutdowns and legal proceedings. The deployment led to a measurable improvement in air quality, evidenced by a reduction of 2.4 μg/m³ in PM2.5 levels during the operational period.

The integration of LiDAR data with complementary environmental datasets enabled precise spatiotemporal analyses, enhancing the efficiency of regulatory enforcement and fostering effective inter-agency collaboration. The results underscore the system’s potential to overcome limitations of conventional point-source monitoring, offering an innovative tool for large-scale industrial air pollution management.

This study highlights the scalability and precision of scanning LiDAR technology as a critical asset for real-time air quality monitoring and regulatory compliance. The findings advocate for broader adoption of this technology in industrial settings globally, emphasizing its ability to address complex environmental challenges and promote sustainable industrial practices.

Acknowledgement: This research was supported by a grant (2023-MOIS-20024324) of Ministry-Cooperation R&D Program of Disaster-Safety funded by Ministry of Interior and Safety (MOIS, Korea) and Climate & Environment Division Scientific Environment Surveillance Team in Gyeonggi-do Province, Korea.

How to cite: Kim, S., Kim, K., Lee, G., Park, J., Oh, S., Sung, M., Kim, S., Jung, Y., Yang, I., Choi, B.-J., Choi, S., and Choi, C.: Real-Time Monitoring of Air Pollution and Detection of Illegal Emissions Using Advanced Scanning LiDAR Technology, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10784, https://doi.org/10.5194/egusphere-egu25-10784, 2025.

EGU25-10819 | Posters on site | GI4.3

Advanced Scanning LiDAR for Real-Time Detection of Wildfires and Industrial Fires 

Kwanchul Kim, Seong-min Kim, Gahye Lee, Jeong-Min Park, Sea-ho Oh, Min-Kyung Sung, Youngmin Noh, Kwonho Lee, Young J. Kim, Woosuk Choi, Sungchul Choi, Changgi Choi, Chun-Sang Hong, Sangcheol Kim, Youndae Jung, Ilkwon Yang, and Byung-Jin Choi

This study introduces the development and application of the advanced scanning LiDAR system, SMART LiDAR MK-II(Samwoo TCS co., Ltd), designed for the early detection of wildfires and industrial fires. Traditional fire detection methods face limitations due to diverse atmospheric conditions, topographical factors, and variability in fire and smoke characteristics. To address these challenges, monitoring systems with spatial resolutions below 30 meters are essential. The SMART LiDAR MK-II employs dual wavelengths (532 nm and 1064 nm) and provides 360° observations with an angular resolution of approximately 3° within a 30-minute interval, enabling the real-time detection of smoke and particulate matter under various environmental conditions.

 

The system was validated through field deployment in the Sihwa Industrial Complex, South Korea, during a fire at an automotive painting factory on July 22, 2024. Positioned at a monitoring height of 55 meters and approximately 20 meters from the fire source, the SMART LiDAR MK-II detected smoke with peak PM10 and PM2.5 concentrations of 724 µg/m³ and 334 µg/m³, respectively. The smoke plume was observed dispersing over 5 km northward, influenced by prevailing winds. Furthermore, the system successfully captured the temporal reduction in particulate matter concentrations following fire suppression, demonstrating its capability to monitor emission dynamics and dispersion patterns.

 

Currently, SMART LiDAR MK-II is undergoing rigorous waterproof and dustproof testing to ensure operational reliability under diverse conditions, with commercialization in progress. This cutting-edge technology represents a significant advancement in LiDAR-based fire detection, offering high spatial resolution, sensitivity, and reliability for real-time monitoring of smoke emissions and atmospheric impacts. The results highlight the transformative potential of SMART LiDAR MK-II to enhance global fire detection and environmental monitoring capabilities.

 

Acknowledgment: This research was supported by a grant (2023-MOIS-20024324) from the Ministry-Cooperation R&D Program of Disaster-Safety funded by the Ministry of Interior and Safety (MOIS, Korea).

How to cite: Kim, K., Kim, S., Lee, G., Park, J.-M., Oh, S., Sung, M.-K., Noh, Y., Lee, K., Kim, Y. J., Choi, W., Choi, S., Choi, C., Hong, C.-S., Kim, S., Jung, Y., Yang, I., and Choi, B.-J.: Advanced Scanning LiDAR for Real-Time Detection of Wildfires and Industrial Fires, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10819, https://doi.org/10.5194/egusphere-egu25-10819, 2025.

EGU25-11218 | ECS | Posters on site | GI4.3

Relationships Between Surface Fluxes and Boundary Layer Dynamics: Statistics at the Land-Atmosphere Feedback Observatory (LAFO) 

Syed Saqlain Abbas, Andreas Behrendt, Oliver Branch, and Volker Wulfmeyer

We studied the convective boundary layer (CBL) processes and surface fluxes long-term statistics by using a combination of two Doppler lidars (DLs) and an eddy-covariance station (EC) at the Land-Atmosphere Feedback Observatory (LAFO), Stuttgart, Germany (Abbas et al., 2024). At LAFO (Späth et al, 2023), one DL is continuously operated in vertical pointing mode, while the second is in six-beam scanning mode, both providing high-resolution data with resolutions of 1 s and 30 m. From this combination of DLs, we derived the profiles of vertical wind variance (Lenschow et al, 2000; Wulfmeyer et al, 2024), horizontal wind variance and turbulent kinetic energy (TKE) as well as CBL depth 𝑧𝑖 (Bonin et al., 2017; Bonin et al., 2018). The surface turbulent fluxes are acquired from an EC station in the agricultural fields of our university ~500 m away from the DLs. Daytime statistics are derived from 20 convective days from May to July 2021 with cloud cover < 40%. In this data set, we found a maximum of the CBL height averaged over all these days ⟨𝑧𝑖⟩ of (1.53 ±0.07) km at 13:30 UTC, which is about 2 hours after local noon. We found counter-clockwise hysteresis patterns between the CBL height and the surface fluxes. In the development phase, these relationships were approximately linear. In the early afternoon, the relationships reached a peak phase with both large fluxes and high values of ⟨𝑧𝑖⟩. At 12:00 UTC, just after local noon, the maximum values of vertical, horizontal, and total TKE were 0.55 m2s-2, 1.26 m2s-2 and 1.71 m2s-2 at heights of (0.30±0.06)⟨𝑧𝑖⟩ , (0.56±0.06)⟨𝑧𝑖⟩, and (0.40±0.06)⟨𝑧𝑖⟩, respectively. In the decay phase in the later afternoon, the relationships show non-linear patterns with larger values of ⟨𝑧𝑖⟩ for the same surface fluxes than in the morning. Furthermore, we analyzed relationships between the vertical and horizontal wind components and total TKE. Also, here, we found non-linear patterns in the three CBL phases.


Abbas, S. S., et al., 2024, https://doi.org/10.5194/egusphere-2024-3878
Späth et al., 2023, https://doi.org/10.5194/gi-12-25-2023
Lenschow et. al., 2000, https://doi.org/10.1175/1520-0426(2000)017<1330:MSTFOM>2.0.CO;2
Wulfmeyer et al., 2024, https://doi.org/10.5194/amt-17-1175-2024
Bonin et. al., 2017, https://doi.org/10.5194/amt-10-3021-2017
Bonin et. al., 2018, https://doi.org/10.1175/JTECH-D-17-0159.1

How to cite: Abbas, S. S., Behrendt, A., Branch, O., and Wulfmeyer, V.: Relationships Between Surface Fluxes and Boundary Layer Dynamics: Statistics at the Land-Atmosphere Feedback Observatory (LAFO), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11218, https://doi.org/10.5194/egusphere-egu25-11218, 2025.

EGU25-11468 | ECS | Posters on site | GI4.3

Network Doppler Lidar for simultaneous multi-parameter observations 

Jan Froh, Josef Höffner, Alsu Mauer, Thorben Mense, Ronald Eixmann, Gerd Baumgarten, Alexander Munk, Sarah Scheuer, and Michael Strotkamp

We present the development progress of our compact multi-field-of-view lidar units for investigating small- to large-scale processes in the atmosphere. Matched narrowband laser and receiver enable precise daylight aerosol measurements with high aerosol visibility and high Doppler wind sensitivity in the troposphere/stratosphere and above. We present recent results with focus on extended measurement capabilities of our transportable systems.

Daylight capable Doppler lidars are complex systems particularly as lidar arrays require compact units with automated functionality. To study the 3-dimensional structure of small- to large-scale atmospheric processes we developed a universal Doppler lidar platform with multiple fields of view. All required technologies are included for studying Mie scattering (aerosols), Rayleigh scattering (air molecules), and resonance fluorescence (potassium atoms) from the troposphere (5 km) to the thermosphere (100 km). We developed unique frequency scanning laser and filter techniques that enable multiple observations (wind, temperature, aerosols, metal density). The combination of narrowband emitter and receiver allow a spectral high resolved characterization of the backscattered Doppler signals with a high wind sensitivity and aerosol visibility. Our current developments focus on enhancing lidar measurement capabilities of multiple parameters together with transferring the technology into industry (Project LidarCUBE) and demonstration of lidar array with enhanced daylight capability (EULIAA – European Lidar Array for Atmospheric Climate Monitoring). We will show recent results of our unique lidar technique with focus on aerosol measurements and more.

How to cite: Froh, J., Höffner, J., Mauer, A., Mense, T., Eixmann, R., Baumgarten, G., Munk, A., Scheuer, S., and Strotkamp, M.: Network Doppler Lidar for simultaneous multi-parameter observations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11468, https://doi.org/10.5194/egusphere-egu25-11468, 2025.

EGU25-11819 | Posters on site | GI4.3

Estimation of optical and microphysical characteristics of contrails using Lidar at SIRTA observatory, Paris 

Cheikh Dione, Jean-Charles Dupont, Karine Caillault, Nicolas Gourgue, Christophe Pietras, and Martial Haeffelin

Contrails are local and thin anthropogenic clouds that are difficult to predict by numerical weather forecasting models. Given their local radiative impact, it is urgent to properly document their characteristics in order to improve their parametrization in weather models and evaluate their contribution to global warming. In the framework of the Climaviation project (Funded by the French Direction Générale de l’Aviation Civile (DGAC)), this study aims to quantify the optical, geometrical and microphysical characteristics of contrails at the SIRTA observatory in Palaiseau, France. We used a co-localised instrumental synergy composed of the Lidar IPRAL (a multichannel raman Lidar), a total sky camera, and aircraft flight altitudes to detect the occurrence of contrails over the site during the 2018-2023 period. Based on three (3) case studies, the particular and molecular integration methods are applied on the Lidar backscatter, to estimate the optical depth of contrails. Vertical profiles of temperature and relative humidity from Trappes radiosoundings are used to characterize the atmospheric conditions classified into three (3) categories of contrail evolution (non-persistent, persistent, and spreading). The results show that the optical thickness of contrails can reach 0.3 for contrails formed in a thick persistent layer. It is lower for contrails developing in a non-persistent layer. During daytime, the contrails contribute to reducing the surface downwelling and upwelling measured shortwave radiation in the order of 218 and 50 W m-2 respectively. Their impact on longwave radiation is relatively negligible.

How to cite: Dione, C., Dupont, J.-C., Caillault, K., Gourgue, N., Pietras, C., and Haeffelin, M.: Estimation of optical and microphysical characteristics of contrails using Lidar at SIRTA observatory, Paris, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11819, https://doi.org/10.5194/egusphere-egu25-11819, 2025.

EGU25-12416 | Orals | GI4.3

Building a Long-Term Cloud Record from Spaceborne Lidars: Bridging CALIOP to ATLID 

Artem Feofilov, Hélène Chepfer, Vincent Noël, and Marius Dahuron

Clouds exert multifaceted radiative effects on Earth's energy budget, serving as both insulators and reflectors of incoming solar radiation while also trapping outgoing infrared radiation. Consequently, clouds contribute to both surface cooling and warming processes, profoundly influencing regional and global climate dynamics. Despite their crucial role in Earth's energy balance, uncertainties persist regarding their feedback mechanisms.

A comprehensive understanding of clouds, including their spatial coverage, vertical distribution, and optical properties, is imperative for accurate climate prediction. Satellite-based observations, particularly those from active sounders, have offered continuous monitoring of clouds with high vertical and horizontal resolution since 2006. However, comparing cloud data from different spaceborne lidars presents challenges due to variations in wavelength, pulse energy, detector type, and local observation times.

This study discusses a methodology aimed at reconciling cloud data derived from several disparate spaceborne lidar platforms: CALIPSO (Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation), which operated from 2006 to 2023; ALADIN/Aeolus (Atmospheric Laser Doppler Instrument), which operated from 2018 to 2023; IceSat-2, operational since 2018; and ATLID/EarthCARE (ATmospheric LIDar), launched last year.

For historical reasons, we use the Scattering Ratio at 532 nm (SR532) as a baseline for defining clouds across all lidars. The numerator contains the Attenuated Total Backscatter at 532 nm (ATB532), while the denominator includes a calculated Attenuated Molecular Backscatter at 532 nm (AMB532), assuming a cloud-free atmospheric profile. For measurements at other wavelengths, we convert the retrieved optical properties to SR532 and ATB532 to enable direct comparison. We demonstrate that this approach facilitates the retrieval of comparable cloud data for CALIOP and ALADIN using real measurements and for CALIOP and ATLID using synthetic measurements.

For lidars overlapping in time, the aforementioned cloud detection parameters can be fine-tuned to ensure a seamless transition between datasets. Collocated data are analyzed with respect to cloud fraction at different latitudes, altitudes, and seasons, and any differences are explored and corrected for, potentially accounting for instrument sensitivity or noise. However, when instruments do not overlap in time, an additional inter-calibrational procedure is necessary. We show how IceSat-2 can serve as a reference to align CALIOP and ATLID cloud datasets.

How to cite: Feofilov, A., Chepfer, H., Noël, V., and Dahuron, M.: Building a Long-Term Cloud Record from Spaceborne Lidars: Bridging CALIOP to ATLID, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12416, https://doi.org/10.5194/egusphere-egu25-12416, 2025.

EGU25-12490 | Orals | GI4.3

 d13C carbon isotopic composition of CO2 in the atmosphere by Lidar 

Fabien Gibert, Dimitri Edouart, Didier Mondelain, Thibault Delahaye, Claire Cénac, and Camille Yver

Our understanding of the global carbon cycle needs for new observations of CO2 concentration at different space and time scales but also would benefit from observations of additional tracers of intra-atmospheric or surface-atmosphere exchanges to characterize sources and sinks. Lidar is a well-known promising technology for this research as it can provide, at the same time, structure of the atmosphere, dynamics and composition of several trace gas concentration. In this framework, a coherent differential absorption lidar (CDIAL) has been developed at LMD to measure simultaneously and separately 12CO2 and 13CO2 isotopic composition of CO2in the atmosphere. It also provides the wind speed along the line of sight of the laser with an additional Doppler ability. This paper investigates the methodology of three wavelengths DIAL in the spectral domain of 2-µm to obtain range-resolved CO2 isotopic ratio d13C. The set-up of the lidar as well as the signal processing is described in details. First atmospheric measurements along three days are achieved in the surface layer above the suburban area of Ecole Polytechnique campus, Palaiseau, France. Typical performances of the instrument (median values along 70h of measurement) with 10 min of time averaging show: (1) a precision around 0.6% for 1.2 km range resolution for 12CO2 mixing ratio (2) a precision around 3.2% for 1.6 km range resolution for 13CO2 mixing ratio. In situ co-located gas analyser measurements are used to correct for biases that are explained neither by the spectroscopic database accuracy nor the signal processing and will need further investigation. Nevertheless, this preliminary study enables to make a useful state of the art for current lidar ability to provide d13C measurements in the atmosphere with respect to geophysical expected anomalies and to predict the necessary performances of a future optimized instrument.

How to cite: Gibert, F., Edouart, D., Mondelain, D., Delahaye, T., Cénac, C., and Yver, C.:  d13C carbon isotopic composition of CO2 in the atmosphere by Lidar, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12490, https://doi.org/10.5194/egusphere-egu25-12490, 2025.

EGU25-12573 | ECS | Orals | GI4.3

Calibration of water vapour Raman lidar using GNSS precipitable water vapour and reanalysis model data 

Arlett Díaz Zurita, Daniel Pérez Ramírez, David Neil Whiteman, Onel Rodríguez Navarro, José Antonio Bravo Aranda, María José Granados Muñoz, Juan Luis Guerrero Rascado, Jesus Abril Gago, Sol Fernández Carvelo, Ana del Águila Pérez, Manuel Antón Martínez, Javier Vaquero Martínez, Alexander Haefele, Giovanni Martucci, Inmaculada Foyo Moreno, José Antonio Benavent Oltra, Lucas Alados Arboledas, and Francisco Navas Guzmán

Water vapour is a crucial and highly variable greenhouse gas in the Earth's atmosphere, which can significantly influence radiative balance, energy transport, and photochemical processes. It can also affect the radiative budget indirectly through cloud formation and by altering the size, shape, and chemical composition of aerosol particles. Accurate and systematic observations are essential for understanding its impacts and improving climate projections. Raman lidar technique is widely used for obtaining water vapour mixing ratio (WVMR) profiles with high vertical and temporal resolution. It relies on Raman scattering from water vapour and nitrogen molecules and is usually calibrated by reference to one or more external measurements of water vapour.

This study presents a hybrid methodology for obtaining high temporal resolution calibration constants for Raman lidar measurements, and posteriorly retrieves high accuracy WVMR profiles. It combines correlative measurements of precipitable water vapour (PWV) for calibrating lidar measurements with Numerical Weather Prediction (NWP) data to reconstruct the profile within the incomplete lidar overlap region. This methodology is applied to the MULHACEN Raman lidar system, operational at UGR station of the University of Granada (Spain) for the long period of 2009-2022. The hybrid method was optimized for the station by selecting Global Navigation Satellite System (GNSS) PWV data as the most appropriate due to its better agreement with correlative radiosondes (R2 of 0.95). Furthermore, the ERA5 model was selected as the most appropriate for reconstructing the incomplete lidar overlap region due to its better temporal and spatial resolution and its accuracy when evaluated against radiosonde data. The advantages of the hybrid calibration methodology are evaluated compared to traditional radiosonde-based methods or PWV data assuming a constant WVMR in the incomplete overlap region. Although all methods generally provide good calibration constants, the hybrid approach presented the best performance, as quantified by an R2 of 0.85, a slope of 0.97, and an intercept of -0.05 g/kg, particularly under conditions where atmospheric layers are not well-mixed. Comparison with radiosonde data revealed excellent agreement, with a mean bias error of -0.11 ± 0.38 g/kg and a standard deviation of 1.04 ± 0.35 g/kg across the entire period and vertical range (0 – 6.0 km agl). The most important result of this study is the ability to continuously evaluate calibration constants during 14 years of MULHACEN operation. The posterior application of the hybrid methodology to all MULHACEN measurements enabled the generation of a comprehensive long time database of WVMR profiles.

How to cite: Díaz Zurita, A., Pérez Ramírez, D., Neil Whiteman, D., Rodríguez Navarro, O., Bravo Aranda, J. A., Granados Muñoz, M. J., Guerrero Rascado, J. L., Abril Gago, J., Fernández Carvelo, S., del Águila Pérez, A., Antón Martínez, M., Vaquero Martínez, J., Haefele, A., Martucci, G., Foyo Moreno, I., Benavent Oltra, J. A., Alados Arboledas, L., and Navas Guzmán, F.: Calibration of water vapour Raman lidar using GNSS precipitable water vapour and reanalysis model data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12573, https://doi.org/10.5194/egusphere-egu25-12573, 2025.

We present a Doppler lidar designed to detect the molecular spectrum characteristics, which are attributed to the Rayleigh-Brillouin scattering, in the atmospheric boundary layer. The suggested system is a continuous-wave, infrared Doppler lidar based on a bi-static transceiver and a coherent in-phase/quadrature detection scheme. For the detection of the features of the Rayleigh-Brillouin spectrum we use fiber-coupled, balanced photodetectors and a digitizer with a 1.6 GHz bandwidth. This broad bandwidth is necessary for the detection of Doppler shifts not only at frequencies of atmospheric winds, but also of the ones corresponding to molecular and acoustic speed that extend over several hundred megahertz. We demonstrate that using this configuration it is possible to detect the molecular Rayleigh-Brillouin spectrum over 30-minute time periods. The observational range of this system is focused on the lower part of the atmosphere (< 200 m) and the objective is to investigate if the resolved features of the Rayleigh-Brillouin spectrum can be related to the temperature, which could lead to the development of a novel vertical profiler of atmospheric temperature.

How to cite: Angelou, N. and Mann, J.: On the measurement of the Rayleigh-Brillouin spectrum and atmospheric temperature using a coherent Doppler lidar, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12657, https://doi.org/10.5194/egusphere-egu25-12657, 2025.

EGU25-12951 | Posters on site | GI4.3

Gravity waves observed by lidar at the center and edge of the Southern polar vortex 

Natalie Kaifler and Bernd Kaifler

Our Rayleigh lidar systems provide temperature profiles up to 100 km altitude at both a site at southern hemisphere mid-latitudes and at South Pole. Very strong orographic gravity waves dominate in the lee of the Southern Andes in winter, a region proximate to the polar vortex edge where strong winds prevail. In contrast, despite being situated within the stable polar vortex core, continuous but weaker gravity waves are observed above Amundsen-Scott station at South Pole. Potential sources for these waves include catabatic winds flowing across the Transantarctic Mountains – which also give rise to polar stratospheric clouds-, polar vortex dynamics, or lateral progagation from mid-latitudes. We present examples of gravity wave measurements and statistical analyses derived from our multi-year, ongoing datasets.

How to cite: Kaifler, N. and Kaifler, B.: Gravity waves observed by lidar at the center and edge of the Southern polar vortex, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12951, https://doi.org/10.5194/egusphere-egu25-12951, 2025.

EGU25-14705 | ECS | Orals | GI4.3

The calibration and validation of XCO2 measured by Lidar onboard DQ-1 

Lu Zhang and Xifeng Cao Cao

Atmospheric carbon dioxide (CO2) is the primary anthropogenic driver of climate change, accounting for more than half of the total effective radiative forcing (ERF). The accurate monitoring of carbon dioxide is essential to study the global carbon cycle and radiation budget on Earth.The Aerosol and Carbon Detection Lidar (ACDL) instrument, as the first space-borne integrated path differential absorption (IPDA) light detection and ranging (Lidar) for XCO2, was successfully launched in April 2022 onboard the DaQi-1 (DQ-1) satellite.During the two years of on-orbit operation, we constantly updated the processing methods, including the spectral broadening of CO2 caused by water vapor, etc. Finally, we calibrated and validated  the CO2 retrieved by DQ-1 usingTCCON and COCOON, and the results showed that the deviation reached the satellite design demand (1ppm).

How to cite: Zhang, L. and Cao, X. C.: The calibration and validation of XCO2 measured by Lidar onboard DQ-1, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14705, https://doi.org/10.5194/egusphere-egu25-14705, 2025.

EGU25-15242 | ECS | Posters on site | GI4.3

A field intercomparison of inter-instrument variability of six co-located Vaisala CL61 lidar-ceilometers 

Dana Looschelders, Andreas Christen, Sue Grimmond, Simone Kotthaus, Jean-Charles Dupont, Daniel Fenner, Martial Haeffelin, and William Morrison

With the advances in ground-based remote sensing technology, measurement networks of automatic aerosol lidar-ceilometers are developing rapidly across Europe and worldwide. Characterising inter-instrument variability of sensors is crucial to assessing uncertainties in observational campaigns, networks, and for data assimilation. It allows the determination of thresholds that need to be exceeded for the detection of meaningful atmospheric differences between observations obtained at different locations (e.g. urban vs rural).

We co-locate six Vaisala CL61 automatic lidar-ceilometers at the SIRTA atmospheric observatory (Palaiseau, France) for a period of ten days to quantify instrument-related differences in several observed variables: profiles of attenuated backscatter and the linear depolarisation ratio (LDR), as well as derived cloud variables, such as cloud base height (CBH) and cloud cover fraction (CCF), and mixed-layer height. Analysing intervals between 5 and 60 min, median absolute differences between sensors are used to quantify inter-instrument uncertainties. For backscatter and LDR, we differentiate between conditions with rain, clear sky, and clouds, respectively.

The agreement between instruments is capable of resolving climatological differences in mesoscale conditions (5 - 50 km, e.g. across cities) for both profile variables and derived cloud variables and layer heights. However, differences exist and can be linked to signal-to-noise ratio (SNR) and atmospheric conditions. The median absolute inter-sensor differences for 15 min aggregation intervals (AD50) are 1.9 % for total CCF (excluding clear sky and fully overcast conditions) and 7.3 m for CBH. Cloud variables agree better for boundary layer clouds where the first (of five) cloud layer < 4 km agl. The mixed-layer height AD50 is 0 m. Median differences smaller than two instrument range gates (9.6 m) highlight the close inter-instrument agreement.

How to cite: Looschelders, D., Christen, A., Grimmond, S., Kotthaus, S., Dupont, J.-C., Fenner, D., Haeffelin, M., and Morrison, W.: A field intercomparison of inter-instrument variability of six co-located Vaisala CL61 lidar-ceilometers, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15242, https://doi.org/10.5194/egusphere-egu25-15242, 2025.

EGU25-15290 | ECS | Orals | GI4.3

AIRflows - a novel airborne Doppler lidar for high resolution wind measurements 

Philipp Gasch, Andreas Wieser, Thomas Feuerle, Franziska Winter, and Christoph Bollig

Wind is a core state variable of the atmosphere. Extending the capabilities of ground-based measurement systems, airborne Doppler lidar (ADL) onboard research aircraft allows for targeted and spatially resolved wind measurements, which are crucial for localized severe weather events or in inaccessible regions such as over water and complex terrain.

A novel ADL system – AIRflows (‘AIRborne fixed-beam lidar fowind measurements‘)  – has been developed by the Karlsruhe Institute of Technology (KIT) in collaboration with scientific and industrial partners during the last two years.
Up to now, ADL systems use a single Doppler lidar attached to a scanner to provide radial velocity measurements under multiple viewing angles. Multiple viewing angles are needed to reconstruct the 3D wind from the unidirectional radial velocity measurements. Due to cost and size reductions of Doppler lidar units over the recent years, it has now become possible to construct an ADL system that uses multiple lidars with fixed-direction beams, instead of a single lidar with a scanning beam. The simultaneous availability of multiple viewing angles brings advantages: Simulation results have demonstrated that a multi-lidar system can achieve approximately one order of magnitude improved spatial wind measurement resolution as well as higher accuracy, compared to existing scanning systems.

This contribution presents the novel AIRflows system developed by KIT. AIRflows implements the novel fixed-beam, multi-lidar concept onboard the TU Braunschweig Cessna F406 research aircraft. The system uses five modified Doppler lidar modules manufactured by Abacus Laser, one pointing nadir and the other four pointing forward, aft, left and right at an elevation of 30° from nadir.
The first flights deploying AIRflows have been successfully completed during summer 2024. Initial analysis demonstrates wind profiles at 100 m spatial resolution, allowing to resolve fine-scale 3D winds inside the PBL for the first time. As part of the tests, flights to the Alps were conducted in preparation for the upcoming international TEAMx campaign. AIRflows measurements across Alpine valleys and crests provide previously unattainable insight into vertical wind and valley circulations in complex terrain. Similarly, AIRflows measurements across a wind farm in the North Sea provide novel vertically resolved insight into wind farm wake behavior.

Overall, AIRflows revolutionizes the field of airborne wind measurements by providing an order of magnitude improved spatial resolution as well as higher measurement accuracy, compared to previously existing ADL.

How to cite: Gasch, P., Wieser, A., Feuerle, T., Winter, F., and Bollig, C.: AIRflows - a novel airborne Doppler lidar for high resolution wind measurements, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15290, https://doi.org/10.5194/egusphere-egu25-15290, 2025.

EGU25-15418 | ECS | Posters on site | GI4.3

Estimation of the Optical properties of Arctic Cirrus Clouds: Insights fromLIDAR measurements and Monte Carlo simulations 

Gopika Gupta, Peter Voleger, Thomas Kuhn, and Janos Stenszky

Cirrus clouds play a critical role in Earth's energy balance by influencing radiative
processes, reflecting incoming solar radiation, and trapping outgoing infrared radiation. In the
Arctic, extreme conditions limit the observational networks and hinder direct measurements.
However, among various remote sensing tools, LIght Detection And Ranging (LIDAR)
emerges as one of a reliable tool for long-term monitoring of cirrus cloud optical properties
over the Arctic region. The extinction coefficient, derived from LIDAR measurements and
essential for evaluating the radiative effects of cirrus clouds, is strongly impacted by the
Multiple Scattering Factor (MSF). In this regard, the present study aims to estimate the MSF
by simulating LIDAR signals using the Monte Carlo method. The input parameters for the
Monte Carlo simulations include the geometry of the atmosphere and optical properties
(including extinction and Mueller matrix). Furthermore, the Mueller matrix is estimated based
on the size distribution and particle shape information acquired through the in-situ measurement
from the Balloon-borne Ice Cloud Particle Imager (B-ICI) instrument. The MSF contribution,
at least in part, depends on the characteristics of the LIDAR, particularly its Field of View. As
a result, new simulations are required, and previous results from older studies cannot be directly
applied.
The photon backscatter information obtained from the Analog and Photon
counting channels of the ground-based LIDAR instrument installed at IRF, Kiruna (68ºN,
20ºE), is utilised to estimate the cirrus cloud's optical properties. To address the instrument’s
non-linear behaviour at higher signal intensities, a glueing procedure is performed to merge the
Analog and the Photon counting signal. The resulting glued signal undergoes multiple
corrections, including background noise subtraction, signal-to-noise ratio enhancement, and
range corrections. The Dynamic Wavelet Covariance Transform (DWCT) technique is
deployed to the corrected LIDAR signal to estimate the cloud top and base altitude information.
Subsequently, an inversion technique incorporating MSF, such as the Sassen method, is chosen
for the current analysis.
The estimated cirrus cloud optical properties using the ground-based LIDAR will
subsequently be validated against EarthCARE’s ATmospheric LIDar (ATLID) satellite
observations. This study enhances the accuracy of cirrus cloud parameterisation, contributing
to improved climate models and a deeper understanding of Arctic cloud-radiative interactions.

How to cite: Gupta, G., Voleger, P., Kuhn, T., and Stenszky, J.: Estimation of the Optical properties of Arctic Cirrus Clouds: Insights fromLIDAR measurements and Monte Carlo simulations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15418, https://doi.org/10.5194/egusphere-egu25-15418, 2025.

In August 2022, China successfully launched the Terrestrial Ecosystem Carbon Inventory Satellite (TECIS). The primary payload of this satellite is an onboard multi-beam lidar system, which is capable of observing aerosol optical parameters on a global scale. This pioneering study used the Fernald forward integration method to retrieve aerosol optical parameters based on the Level 2 data of the TECIS, including the aerosol depolarization ratio, aerosol backscatter coefficient, aerosol extinction coefficient, and aerosol optical depth (AOD). The validation of the TECIS-retrieved aerosol
optical parameters was conducted using CALIPSO Level 1 and Level 2 data, with relative errors within 30%. A comparison of the AOD retrieved from the TECIS with the AERONET and MODIS AOD products yielded correlation coefficients greater than 0.7 and 0.6, respectively. The relative error
of aerosol optical parameter profiles compared with ground-based measurements for CALIPSO was within 40%. Additionally, the correlation coefficients R2 with MODIS and AERONET AOD were approximately between 0.5 and 0.7, indicating the high accuracy of TECIS retrievals. Utilizing the TECIS retrieval results, combined with ground air quality monitoring data and HYSPLIT outcomes, a typical dust transport event was analyzed from 2 to 7 April 2023. The results indicate that dust was transported from the Taklamakan Desert in Xinjiang, China, to Henan and Anhui provinces, with a gradual decrease in the aerosol depolarization ratio and backscatter coefficient during the transport process, causing varying degrees of pollution in the downstream regions. This research verifies the accuracy of the retrieval algorithm through multi-source data comparison and demonstrates the potential application of the TECIS in the field of aerosol science for the first time. It enables the fine-scale regional monitoring of atmospheric aerosols and provides reliable data support for the three-dimensional distribution of global aerosols and related scientific applications.

How to cite: Chen, B.: The First Validation of Aerosol Optical Parameters Retrieved from the Terrestrial Ecosystem Carbon Inventory Satellite (TECIS) and Its Application, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15492, https://doi.org/10.5194/egusphere-egu25-15492, 2025.

EGU25-16068 | ECS | Orals | GI4.3

Comprehensive Study of Cloud Characteristics over a High Altitude Station - Leh, India using Ground-Based Lidar and Satellite Observations 

Ruchita Shah, Som Sharma, Dharmendra Kamat, Shantikumar Ningombam, Dorje Angchuk, and Rohit Srivastava

A rise of approximately 1°C in global average temperature is influencing sea surface temperature, sea-level, intensity of storms, frequency and severity of hydro-meteorological extreme events. Such effects are comparatively more pronounced in tropical and sub-tropical zones, wherein Leh-Ladakh region of Indian subcontinent, is peculiar and characterized by extreme weather conditions. The present work unravels the cloud characteristics over the Leh region using ground-based ceilometer lidar (3255 m above mean sea level), remote-sensing, and reanalysis data sets for one-year (September 2022–August 2023). Variations in cloud base height (CBH) was observed with lidar, enabling the measurement of CBH up to three distinct layers, designated as CBH1, CBH2, and CBH3, respectively. This study reveals distinct seasonal and altitudinal variations in CBH, with cloud occurrence frequencies peaking during the pre-monsoon (67.94%) and monsoon (98%) seasons, reflecting the onset and active phases of the Indian summer monsoon. Month of July was recorded with the highest prevalence of multi-layered clouds (84.03%), which includes triple-layered clouds (CBH3, 42.13%) dominating over double-layered (CBH2, 25.98%) and single-layered (CBH1, 15.92%) clouds. Seasonal analysis showed a dominance of mid-level clouds (~3–6 km, 77.53%), while high-level clouds (~6–18 km, 4.43%) were less frequent. Altostratus and altocumulus clouds were particularly prominent across all seasons, with their variability linked to topographic and climatic factors. The ceilometer's high-resolution measurements captured the temporal dynamics of CBH, which aligned with satellite and reanalysis data, demonstrating the value of ground-based instruments in complementing remote sensing technologies. These findings provide valuable insights into cloud dynamics and their role in extreme weather events such as cloudbursts and intense rainfall, which are increasingly frequent in the Himalayan region. By improving our understanding of cloud–precipitation interactions, this study offers critical information for enhancing weather forecasting, informing rainfall prediction models, and supporting climate adaptation strategies in climatically vulnerable high-altitude regions.   

How to cite: Shah, R., Sharma, S., Kamat, D., Ningombam, S., Angchuk, D., and Srivastava, R.: Comprehensive Study of Cloud Characteristics over a High Altitude Station - Leh, India using Ground-Based Lidar and Satellite Observations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16068, https://doi.org/10.5194/egusphere-egu25-16068, 2025.

EGU25-16402 | Posters on site | GI4.3

1.65 µm CH4 ground-based differential absorption lidar measurements in the atmosphere 

Dimitri Edouart, Fabien Gibert, and Claire Cénac

Methane (CH4) is the second anthropogenic greenhouse gas (GHG) in the atmosphere that contributes to the global warming after CO2. If the methane emissions have a unique sink by OH oxidation, the various different sources, both anthropogenic (around 2/3) and natural, make complex the understanding of its atmospheric concentration. On the anthropogenic side (mainly gas exploitation and burning) it is fundamental to have a tool to verify inventories at different scales (from local methanizer to megacity) and prevent production network leakage in the atmosphere. As for surface-atmosphere exchanges of CO2, it is fundamental to study at different scales the spatial pattern and magnitude of the natural CH4 sources (biogenic anaerobic degradation of organic matter in wetlands, landfill and waste, livestock, rice cultivation, thermite, geological sources) and to understand their evolution with the global warming.

Lidar has an important role to play in such topic as it can make: (i) a 3D mapping of CH4 concentration in anthropogenic plumes, (ii) vertical profiles to study transport processes in the atmosphere, (iii) even measure direct flux and (iv) provide CH4 Earth global measurements from a space platform as it will be for MERLIN CH4 integrated path differential absorption lidar CNES/DLR ongoing mission.

A new ground-based Differential Absorption Lidar (DIAL) for atmospheric methane (CH4) profiling has been developed at LMD. The lidar emitter relies on a new hybrid fibered/bulk Er:YAG laser that delivers dual On/Off 8 mJ/ 300 ns pulses at a repetition frequency of 1 kHz in the methane line triplet at 1645.55 nm and out of at 1645.3 nm. It is associated with a direct detection receiver with a 50cm diameter telescope, a 2-nm linewidth interference optical filter, a near infrared photomultiplier (PMT) and a data acquisition and real time signal processing system working both in analogic and photon counting mode depending the application. First horizontal and vertical measurements in the atmosphere have been achieved and compared with in situ sensor and will be presented at the conference.

How to cite: Edouart, D., Gibert, F., and Cénac, C.: 1.65 µm CH4 ground-based differential absorption lidar measurements in the atmosphere, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16402, https://doi.org/10.5194/egusphere-egu25-16402, 2025.

EGU25-16832 | ECS | Orals | GI4.3

Integration of Doppler Wind Lidars in E-Profile wind profiling network 

Eric Sauvageat, Rolf Rüfenacht, Maxime Hervo, Myles Turp, Markus Kayser, Ronny Leinweber, Volker Lehmann, Steven Knoop, Alexander Gohm, and Alexander Haefele

E-Profile is the EUMETNET Programme coordinating the measurements of vertical profiles of wind, aerosols and clouds from radars and lidars in Europe. The E-Profile wind network provides near real-time vertical profiles of wind from weather radars and dedicated wind profilers with the main goal to promote the usability of these data for operational meteorology and provide expertise to both the data provider and the end-user.

Ground-based scanning Doppler Wind Lidars (DWLs) are capable of measuring wind profiles in the atmospheric boundary layer (ABL) at a high spatial and temporal resolution and they have the potential to improve the short-term wind forecast. With the availability of commercial DWLs in the last decade, many meteorological services and scientific institutions are now operating such instruments or are planning to do so in the future in Europe.

To extend the benefit of these observations and promote data sharing, these instruments have recently been integrated in E-Profile wind profiling network. Using an open-source code developed at the Deutscher Wetterdienst (DWD), instrument’s data from different manufacturers are processed in a harmonized way to provide 10 minutes averaged wind profiles in the ABL. Data are converted to BUFR and distributed in near real-time on the Global Telecommunication System (GTS), making them available globally for data assimilation. At the moment, 12 DWLs from 4 European countries are being processed operationally and more instruments are expected to join the network in 2025.

Here, we present the integration of DWL into the E-Profile wind network, its associated challenges and the requirements for the scan strategies. We also show comparisons at different sites against other wind profiling instruments (e.g. radar wind profilers) and against model data. Finally, we also discuss the future improvements to the network.

How to cite: Sauvageat, E., Rüfenacht, R., Hervo, M., Turp, M., Kayser, M., Leinweber, R., Lehmann, V., Knoop, S., Gohm, A., and Haefele, A.: Integration of Doppler Wind Lidars in E-Profile wind profiling network, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16832, https://doi.org/10.5194/egusphere-egu25-16832, 2025.

EGU25-16880 | ECS | Posters on site | GI4.3

The desert dust impact on the Boundary Layer in the Atlantic 

Ioanna Tsikoudi, Eleni Marinou, Maria Tombrou, Eleni Giannakaki, Emmanouil Proestakis, Konstantinos Rizos, and Vassilis Amiridis

The study investigates the dynamics of the Boundary Layer (BL) over the Atlantic Ocean, with a focus on the region surrounding Cabo Verde, using a combination of ground-based PollyXT lidar, satellite lidar data from Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations (CALIPSO), radiosondes, and European Centre for Medium-Range Weather Forecasts (ECMWF) model output. The comparison of CALIPSO lidar profiles with ECMWF reanalysis revealed strong correlations for BL top over open ocean regions but less agreement in dust-affected areas closer to the African continent. In these regions, satellite lidar indicated higher BL tops than those estimated by ECMWF, likely due to the existence of high of aerosol concentrations, which play a crucial role in shaping dynamics. Observations in Cabo Verde highlight distinctive Marine Atmospheric Boundary Layer (MABL) characteristics, such as limited diurnal evolution, but also show the potential for BL heights to reach up to 1 km, driven by factors like strong winds that increase mechanical turbulence. Additionally, this study illustrates the challenges in accurately determining the BL height using lidar and radiosondes, examining cases with strong inversions that prevent vertical mixing, but also weaker inversions that allow for the penetration of dust particles within BL. Integrating multiple observational sources and techniques is essential for validating remote sensing data and enhancing BL characterizations. The findings underscore the complex interactions between marine and dust-laden air masses over the Atlantic, which are essential for understanding the dynamic processes in aerosol-cloud interactions.

How to cite: Tsikoudi, I., Marinou, E., Tombrou, M., Giannakaki, E., Proestakis, E., Rizos, K., and Amiridis, V.: The desert dust impact on the Boundary Layer in the Atlantic, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16880, https://doi.org/10.5194/egusphere-egu25-16880, 2025.

EGU25-17781 | ECS | Orals | GI4.3

Using the ESA eVe reference lidar system for the cal/val of lidar instruments onboard ESA satellite missions 

Peristera Paschou, Eleni Marinou, Kallopi Artemis Voudouri, Nikolaos Siomos, Antonis Gkikas, Jonas von Bismarck, Thorsten Fehr, and Vassilis Amiridis

The eVe lidar is ESA’s ground reference lidar system for the calibration and validation (cal/val) of ESA satellite missions. eVe is a combined linear/circular polarization lidar with Raman capabilities operating at 355 nm and deriving the profiles of the optical properties of aerosols and thin clouds, namely the particle backscatter and extinction coefficients, the lidar ratio, and the linear and circular depolarization ratios. The system is implemented in a dual-laser/dual-telescope configuration and it can be rotated to perform lidar measurements using different pointing geometries. As such, eVe can simultaneously reproduce the operation of any lidar system that uses linearly (e.g traditional polarization lidars; ATLID onboard EarthCARE mission) or circularly (e.g. ALADIN lidar onboard Aeolus mission) polarized emission.

The eVe lidar has been deployed in ASKOS, the ground-based component of the Joint Aeolus Tropical Atlantic Campaign in Cabo Verde (2021 and 2022), for performing targeted circular polarization lidar measurements for the validation of the Aeolus aerosol products (i.e. the Aeolus L2A products). The eVe-Aeolus comparisons reveal that the Aeolus co-polar backscatter coefficient is the most accurate L2A product followed by the noisier particle extinction coefficient with the larger discrepancies for the Aeolus profiles to be observed in lower altitudes where the aerosol load is larger. The Aeolus co-polar lidar ratio is the noisiest L2A product with the largest discrepancies from the corresponding eVe profiles. Currently the eVe lidar is under upgrade with main components of enabling the profiling of water vapor mixing ratio and extending the retrieval of the extinction coefficient towards daytime conditions, aiming to further enhance its measuring capabilities as well as to meet the requirements for the cal/val of the ATLID lidar products onboard EarthCARE mission which is currently in orbit. After the upgrade, eVe lidar will perform targeted measurements during the nearest EarthCARE overpasses from eVe’s location for the evaluation of the ATLID L2A products.

Acknowledgements:

This research is financially supported by the PANGEA4CalVal project (Grant Agreement 101079201) funded by the European Union and the “Best practice protocol for validation of Aerosol, Cloud, and Precipitation Profiles” ESA project (ACPV; Contract no. 4000140645/23/I-NS). The ASKOS campaign was funded by an ESA project (Contract no. 4000131861/20/NL/IA) and the acquired dataset can be accessed via https://evdc.esa.int/publications/askos-campaign-dataset/. The eVe lidar upgrade and the deployment for the cal/val of EarthCARE products are funded by an ESA project (Contract no. 4000146416/24/NL/FFi).

How to cite: Paschou, P., Marinou, E., Voudouri, K. A., Siomos, N., Gkikas, A., von Bismarck, J., Fehr, T., and Amiridis, V.: Using the ESA eVe reference lidar system for the cal/val of lidar instruments onboard ESA satellite missions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17781, https://doi.org/10.5194/egusphere-egu25-17781, 2025.

EGU25-18284 | ECS | Orals | GI4.3

Assessment of horizontally-oriented ice crystals with a combination of multiangle polarization lidar and cloud Doppler radar 

Zhaolong Wu, Patric Seifert, Yun He, Holger Baars, Haoran Li, Cristofer Jimenez, Chengcai Li, and Albert Ansmann

The orientation of ice crystals plays a significant role in determining their radiative and precipitating effects, horizontally oriented ice crystals (HOICs) reflect up to ~40 % more short-wave radiation back to space than randomly oriented ice crystals (ROICs). This study for the first time introduces an automatic pixel-by-pixel algorithm for HOIC identification using a combination of ground-based zenith- and 15-degree off-zenith-pointing polarization lidars. The lidar observations provided high-resolution cloud phase information. The data were collected in Beijing over 354 days in 2022. A case study from 13 October 2022 is presented to demonstrate the effectiveness and feasibility of the detection method. The synergy of lidars and collocated Ka-band cloud radar, radiosonde, and ERA5 data provide phenomenological insights into HOIC events. While cloud radar Doppler velocity data allowed the estimation of ice crystal size, Reynolds numbers, and turbulent eddy dissipation rates, corresponding environmental and radar-detected variables are also provided. HOICs were present accompanying with weak horizontal wind of 0–20 ms−1 and relatively high temperature between −8 °C to −22 °C. Compared to the ROICs, HOICs exhibited larger reflectivity, spectral width, turbulent eddy dissipation rate, and a median Doppler velocity of about 0.8 ms−1. Ice crystal diameter (1029 µm to 1756 µm for 5th and 95th percentiles) and Reynolds numbers (28 to 88 for 5th and 95th percentiles) are also estimated with the help of cloud radar Doppler velocity using an aerodynamic model. One interesting finding is that the previously found switch-off region of the specular reflection in the region of cloud base shows a higher turbulence eddy dissipation rate, probably caused by the latent heat released due to the sublimation of ice crystals in cloud-base region. The newly derived properties of HOICs have the potential to aid to derive the likelihood of their occurrence in output from general circulation models (GCMs) of the atmosphere.

How to cite: Wu, Z., Seifert, P., He, Y., Baars, H., Li, H., Jimenez, C., Li, C., and Ansmann, A.: Assessment of horizontally-oriented ice crystals with a combination of multiangle polarization lidar and cloud Doppler radar, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18284, https://doi.org/10.5194/egusphere-egu25-18284, 2025.

EGU25-18566 | Posters on site | GI4.3

Enhancing lidar aerosol typing schemes: a lidar/photometer synergy 

Nikolaos Papagiannopoulos, Michail Mytilinaios, Aldo Amodeo, Giuseppe D'Amico, Pilar Gumà-Claramunt, Christina Anna Papanikolaou, and Lucia Mona

In this study we present a synergistic approach between lidar and photometer to separate volcanic ash and desert dust and, ultimately, to enhance lidar-based aerosol typing schemes. Typically, the lidar depolarization ratio measurements can be used to distinguish dust and ash with ash depolarization ratio reaching higher values. However, the variability of aerosol depolarization ratio makes it difficult to use it in automatic typing techniques. The imaginary part of refractive index when using in situ data shows stronger absorption than mineral dust; therefore, here, we make use of microphysical AERONET data to define the two aerosol classes (i.e., ash/dust). Then, trivariate Mahalanobis distance is estimated based on the real and imaginary parts of the refractive index and the single scattering albedo for any given AERONET measurement and the type is assigned. This information is then passed on in lidar aerosol typing algorithms and the aerosol type is allocated in the vertical dimension. The methodology is applied to the Potenza ACTRIS site in Italy during an intense desert dust event where an AERONET photometer and an ACTRIS lidar are collocated.

How to cite: Papagiannopoulos, N., Mytilinaios, M., Amodeo, A., D'Amico, G., Gumà-Claramunt, P., Papanikolaou, C. A., and Mona, L.: Enhancing lidar aerosol typing schemes: a lidar/photometer synergy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18566, https://doi.org/10.5194/egusphere-egu25-18566, 2025.

EGU25-19403 | Orals | GI4.3 | Highlight

Forecasting Climate Adaptation Through Cirrus Cloud Radiative Forcing Analysis Using 20 Years of MPLNET Lidar Measurements 

Simone Lolli, Andreu Salcedo-Bosch, Jasper R. Lewis, Erica K. Dolinar, James R. Campbell, and Ellsworth J. Welton

Cirrus clouds play a critical role in Earth's radiation budget and are key to understanding and forecasting climate adaptation in response to global warming. Leveraging 20 years of high-resolution lidar data from NASA's MPLNET network, we analyze and forecast cirrus cloud radiative forcing with the aim of projecting how the climate system will adapt to changing atmospheric conditions. Using ensemble learning methods, we simulate the monthly radiative impacts of cirrus clouds, emphasizing their variability and feedback mechanisms. The study also integrates future climate scenarios under shared socio-economic pathways ( CMIP6SSP2-4.5 and SSP5-8.5) to explore potential shifts in regional climate patterns driven by cirrus cloud interactions. Results highlight how increased temperatures and altered precipitation regimes may influence the climate's adaptive processes, particularly in regions currently sensitive to radiative forcing fluctuations. This research underscores the importance of long-term lidar data for advancing climate adaptation modeling and identifying critical atmospheric feedbacks.

[1] Lolli, S., 2023. Machine Learning Techniques for Vertical Lidar-Based Detection, Characterization, and Classification of Aerosols and Clouds: A Comprehensive Survey. Remote Sensing15(17), p.4318.

How to cite: Lolli, S., Salcedo-Bosch, A., Lewis, J. R., Dolinar, E. K., Campbell, J. R., and Welton, E. J.: Forecasting Climate Adaptation Through Cirrus Cloud Radiative Forcing Analysis Using 20 Years of MPLNET Lidar Measurements, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19403, https://doi.org/10.5194/egusphere-egu25-19403, 2025.

EGU25-19850 | Orals | GI4.3

Estimating Planetary Boundary Layer Height Using CALIPSO Lidar Data: A Machine Learning Approach 

Francesc Rocadenbosch, Andreu Salcedo-Bosch, and Simone Lolli

The planetary boundary layer height (PBLH) is a critical atmospheric parameter influencing air quality, pollutant dispersion, and weather forecasting. Traditional methods for PBLH retrieval rely on radiosondes and ground-based sensors, but their spatial and temporal coverage is limited. In this study, we present a novel application of Random Forest (RF) machine learning to estimate PBLH using lidar measurements from the CALIPSO satellite's Level 1 data spanning a decade. Our RF model is trained with an extensive dataset of radiosonde-derived PBLH values coinciding with CALIPSO overpasses. This approach leverages CALIOP's lidar backscatter profiles to achieve robust performance (R² = 0.6, RMSE = 333.59 m) across a range of atmospheric conditions, including cloudy and dust-laden scenarios, without requiring atmospheric typing or ancillary data. The results surpass state-of-the-art methods in global applicability and accuracy, offering improved spatial and temporal resolution of PBLH estimates. We also discuss the model's performance variations between day- and nighttime scenarios and highlight challenges, such as data bias and surface reflection contamination, which inform future model refinements. This study underscores the potential of integrating machine learning and lidar remote sensing for advancing atmospheric science [1-2].

 

REFERENCES

[1] S. Lolli, W. Y. Khor, M. M. Z. Matjafri, and H. S. Lim, "Monsoon season quantitative assessment of biomass burning clear-sky aerosol radiative effect at surface by ground-based lidar observations in Pulau Pinang, Malaysia in 2014," Remote Sensing, vol. 11, no. 22, 2019.

[2] C. Sivaraman, S. McFarlane, E. Chapman, M. Jensen, Toto, S. Liu, and M. Fischer, Planetary Boundary Layer Height (PBL) Value Added Product (VAP): Radiosonde Retrievals, Tech. Rep., DOE Office of Science Atmospheric Radiation Measurement (ARM) Program, United States, Aug. 2013.

ACKNOWLEDGEMENTS
This research is part of the project PID2021-126436OB-C21 funded by Ministerio de Ciencia e Investigación (MCIN)/Agencia Estatal de Investigación (AEI)/ 10.13039/501100011033 y FEDER “Una manera de hacer Europa” and part of the PRIN 2022 PNRR, Project P20224AT3W funded by Ministero dell’Universit`a e della Ricerca. The European Commission collaborated under projects H2020 ATMO-ACCESS (GA-101008004) and H2020 ACTRIS-IMP (GA-871115).

How to cite: Rocadenbosch, F., Salcedo-Bosch, A., and Lolli, S.: Estimating Planetary Boundary Layer Height Using CALIPSO Lidar Data: A Machine Learning Approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19850, https://doi.org/10.5194/egusphere-egu25-19850, 2025.

EGU25-20478 | ECS | Orals | GI4.3

Proof-of-Concept of a Short-Range High Spectral Resolution Lidar using a Compact High Repetition Rate Fiber Laser 

Manuela Hoyos Restrepo, Romain Ceolato, and Yoshitaka Jin

In recent years, several climate and air quality applications have required to understand the impact of aerosols close to their source, leading to the development of novel Short-Range Elastic Backscatter Lidars (SR-EBLs), which enable measuring the radiative properties of aerosols at high spatiotemporal resolutions (<10cm, 1s) in the short-range (3 to 500m). However, the elastic lidar equation is an ill-posed problem, having one equation for two atmospheric variables: the backscatter β(r) and extinction α(r) coefficients. Solving this equation requires assuming a value for the lidar ratio, i.e., a linear relationship between β and α, reducing the accuracy of the retrievals. Advanced lidar techniques, like the High Spectral Resolution Lidar (HSRL), measure molecular and particle scattering separately. Having a direct measurement of the molecular component allows for solving the lidar problem without assumptions about the lidar ratio. However, the existing atmospheric HSRLs cannot perform short-range measurements because i) they are usually blind in the first hundredths of meters (overlap restrictions), and ii) they prioritize spectral performance using ultranarrow band (and thus long-pulse) lasers, resulting in an insufficient spatiotemporal resolution.

This work presents a proof-of-concept of a Short-Range High Spectral Resolution Lidar (SR-HSRL) optimized for aerosol characterization in the first kilometer of the atmosphere. This SR-HSRL uses a compact high-repetition rate fiber laser source with a 300 MHz linewidth and 5 ns pulse length. Since these two parameters are inversely proportional, and both are required for performing SR-HSRL measurements, a compromise had to be found to optimize the overall performance. The main challenge was to prove that, despite its relatively large linewidth, this laser has a satisfactory spectral performance so that it can be used for future implementations of the short-range HSRL. We chose this model after evaluating several laser sources because it has the right compromise between pulse length, linewidth, spectral stability, and size. The laser housing is 270 x 270 x 40 mm and weighs 2.9 kg, making it ideal for future integration on a portable short-range HSRL system.

In the receiver part, a 10:90 beam splitter transmits 10% of the backscattered light to the total channel and reflects 90% of it to the HSR channel. A 40-cm-long iodine cell is used as the spectral filter for separating the Mie and Rayleigh aerosol components. We used two thermoelectrically cooled SiPM Multi-Pixel Photon Counter (MPPC) sensors and a 160MHz analog-to-digital converter to measure the signals. The spatiotemporal resolution, limited by the acquisition system, is 7.5 m and 1 s.

To test the lidar, a two-day measurement campaign was performed at NIES in Tsukuba, Japan, in July 2024. We demonstrate that, despite having a relatively large laser linewidth, we can successfully remove the Mie aerosol component, retrieving aerosol backscatter coefficient profiles from as low as 80 m. We also compare the HSRL retrieval method to a non-conventional forward Fernald inversion method previously reported for SR-EBL. We found that the forward method normally sub-estimates β (up to 30% discrepancy) in aerosol layers and overestimates it in cloud zones (60 to >100% difference).

How to cite: Hoyos Restrepo, M., Ceolato, R., and Jin, Y.: Proof-of-Concept of a Short-Range High Spectral Resolution Lidar using a Compact High Repetition Rate Fiber Laser, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20478, https://doi.org/10.5194/egusphere-egu25-20478, 2025.

EGU25-21151 | Orals | GI4.3

Simulation and assessment of spaceborne hybrid Doppler wind lidar 

Songhua Wu, Guangyao Dai, Wenrui Long, Kangwen Sun, Xiaochun Zhai, Na Xu, and Xiuqing Hu

Accurately measuring wind field is crucial for studying the dynamical structure and evolutionary characteristics of the atmosphere, as well as heat-momentum-matter exchange and balance. According to the World Meteorological Organization (WMO), global observation of the 3D wind field is the primary factor for improving the accuracy of numerical weather prediction. Due to the absence of aeronautical data, meteorological observation and forecasting capabilities are notably deficient in sparsely populated areas, the southern hemisphere, the polar regions, and the vast oceans. Spaceborne Doppler wind lidar has become an important instrument for observing the vertical profile of the global wind field, with the successful operation of Aeolus. The third generation of FengYun polar-orbiting meteorological satellites are initially designed to develop a dual-system Doppler wind measurement lidar technology programme that integrates direct and coherent detection lidar, making full use of the observational advantages of the two methods to detect the global wind field with high resolution. Incoherent detection is used in the middle and upper troposphere and lower stratosphere, where molecules scatter strongly. Coherent detection is used for the observation of the middle and lower troposphere and boundary layer. This research analyses the key parameters of the spaceborne hybrid wind lidar for future satellite missions. The incoherent detection module operates at 355 nm and uses the dual-edge detection technique based on Fabry?Pérot etalon. And the coherent detection module uses heterodyne detection technique operating at 1064 nm. This paper presents a simulation model for wind measurement lidar that realizes gridded atmospheric parameters, scanning observation, and forward-inversion simulation. And a method for detecting horizontal wind field based on dual-beam observation was developed to ensure the response of the lidar for wind speed detection in both meridional wind component and zonal wind component.

How to cite: Wu, S., Dai, G., Long, W., Sun, K., Zhai, X., Xu, N., and Hu, X.: Simulation and assessment of spaceborne hybrid Doppler wind lidar, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21151, https://doi.org/10.5194/egusphere-egu25-21151, 2025.

EGU25-21533 | Posters on site | GI4.3

Cloud Condensation Nuclei (CCN) and Ice Nucleating Particles (INP) conversion factors based on Thessaloniki AERONET station 

Eleni Giannakaki, Karageorgopoulou Archontoula, Georgoulias Aristeidis, and Koutounidis Ioannis

Several studies [1,2] have shown the potential of polarization lidar to provide vertical profiles of aerosol parameters from which cloud condensation nuclei (CCN) and ice-nucleating particles (INP) number concentrations can be retrieved. The results are based on reliable of conversion factors between aerosol optical thickness and column-integrated particle size distribution based on Aerosol Robotic Network (AERONET) photometer observations. A crucial point regarding the efficacy of aerosol particles to act as CCN or INP depends on aerosol type.

AERONET Inversion Data (Level 1.5) for Thessaloniki station were analyzed over the period 2006-2021. Following ‎[1,2], the Ångström exponent was used to separate the particles into pollution (AE > 1.6) and dust (AE < 0.5) dominated cases. To obtain a better classification of aerosols we utilize aerosol typing from CALIPSO. Only cases which are classified as either purely dust or polluted continental aerosols within 100km from Thessaloniki are selected. The Aerosol Optical Depth (AOD) at 440 nm and the Ångström exponent (AE) 440-870 were used to calculate the AOD at 532 nm, while the AOD at 1020 nm and the AE between 870-1020 nm were used to estimate the AOD at 1064 nm. The particle volume size distribution is derived for 22 discrete radius points, spaced logarithmically at equidistant intervals. The particle number concentration (n) for each radius interval is calculated by dividing the volume concentration by the particle volume and multiplying by the spectral integral width of 0.2716. The column value of n60 is the sum of number concentrations for radius classes 2 to 22 (>57 nm), while n100 is the sum for radius classes 4 to 22 (>98 nm). The INP-relevant column n250 is the sum of intervals 8–22 plus the mean of intervals 7 and 8, while n290 the sum of 8-22. To obtain particle extinction coefficient σ (or sigma) and n60, the AOD at 532 nm and the column n60 are divided by 1000 m. For urban particles, n60 (reservoir of CCN) and n250 (reservoir of INP) were used, while n100 (CCN) and n250 (INP) were used for dust particles. Following CALIPSO aerosol typing dust conversion factors was found equal to c100= 24.3±7.0 Mm cm-3, xd=0.78 ± 0.13 and c250= 0.30±0.03 Mm cm-3, while for polluted continental particles, were c60= 31.4 ± 9.0 Mm cm-3, xc= 0.94 ± 0.12 and c290= 0.089±0.002 Mm cm-3.

 

References:

[1] Mamouri, R.E. and Ansmann, A. Potential of polarization lidar to provide profiles of CCN- and INP-relevant aerosol parameters. Atmos. Chem. Phys. 2016, 16, 5905–5931. doi:10.5194/acp-16-5905-2016

[2] Georgoulias, A.; Marinou, E.; Tsekeri, A.; Proestakis, E.; Akritidis, D.; Alexandri, G.; Zanis, P.; Balis, D.; Marenco, F.; Tesche, M. and Amiridis, V. A First Case Study of CCN Concentrations from Spaceborne Lidar Observations. Remote Sens. 2020, 12, 1557. doi:10.3390/rs12101557

 

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

How to cite: Giannakaki, E., Archontoula, K., Aristeidis, G., and Ioannis, K.: Cloud Condensation Nuclei (CCN) and Ice Nucleating Particles (INP) conversion factors based on Thessaloniki AERONET station, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21533, https://doi.org/10.5194/egusphere-egu25-21533, 2025.

EGU25-21736 | Orals | GI4.3

Simultaneous observations of meteoric Ca and Ca+ by employing the Ti:sapphire-laser-based resonance-scattering Ca/Ca+ lidar 

Masayuki Katsuragawa, Mitsumu K. Ejiri, Ayaka Hashimoto, Sota Kobayashi, Sayako Miyoshi, Hikaru Miyagi, Chiaki Ohae, and Takuji Nakamura3

The upper atmosphere located at an altitude of 80 - 120 km above the ground is a crucial region for comprehensively understanding the behavior of Earth's entire atmosphere, because it is the region where the atmosphere transitions from neutral to ionospheric. In this transitional region, meteoroids are continually supplying metallic atoms and ions. The resonant-scattering lidar, which emits laser beams from the ground and then detect on the ground again how much atoms and ions cause resonant scattering of the laser radiations, is one of the significant measurement methods of observing such transitional region. While Fe and Na are selected as the major targets, we have focused on Ca and have developed a specific lidar system to detect it. This is because Ca has uniquely preferable resonance transitions for neutral atoms and ions (Ca: 422.7918 nm and Ca+: 393.4770 nm) for performing lidar measurements from the ground. The core of the developed resonant-scattering Ca/Ca+ lidar system is the injection-locked Ti:sapphire solid-state laser, which has the remarkable ability to simultaneously emit the two laser beams from a single resonator at a variety of combinations of two wavelengths, including the above resonant transitions of neutral Ca and Ca+.
    Here, we report on the first results of the long-term observations, where the developed resonant-scattering Ca/Ca+ lidar system was operated for an entire night. The averaged laser power, time resolution, and altitude resolution of the Ca/Ca+ lidar system are set to 0.2 W, 30 s, and 15 m, respectively, for Ca, and 0.4 W, 30 s, and 30 m , respectively, for Ca+ in this operation. Both neutral Ca and Ca ions distributed in the identical spatio-temporal regions could be measured in detail over an entire night. It was clearly observed that the neutral Ca and Ca ions had almost the same spatio-temporal structures with complex time and space dependences in the main layer at an altitude of 80 - 100 km, and Ca ions also had an additional high-density thin layer with a few kilometers deep at the highest altitude in the main layer. This high-density layer of Ca ions, which was not seen with the neutral Ca, suggests that it is to be related to the sporadic E layer. In our presentation, we will also report on the progress of this ongoing project.

How to cite: Katsuragawa, M., Ejiri, M. K., Hashimoto, A., Kobayashi, S., Miyoshi, S., Miyagi, H., Ohae, C., and Nakamura3, T.: Simultaneous observations of meteoric Ca and Ca+ by employing the Ti:sapphire-laser-based resonance-scattering Ca/Ca+ lidar, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21736, https://doi.org/10.5194/egusphere-egu25-21736, 2025.

EGU25-3236 | ECS | Posters on site | GI4.4

Challenges and Opportunities with Soil Moisture Measurement in Ireland using Cosmic-Ray Neutron Sensing: Examples from an agriculture and a forest site 

Haleh Karbala Ali, Klara Finkele, Rafael Rosolem, Jonathan Evans, Martin Schrön, Brian Tobin, and Eve Daly

Field-scale Soil Moisture (SM) is an important variable to derive and study agriculture, plant growth, nutrient management, water quality and management, soil carbon sequestration, groundwater availability, flood forecasting, forest fire risk, land surface models and is an Essential Climate Variable (ECV). Field-scale SM estimates are vital due to small scale soil heterogeneities and can fill the gap between the traditional in-situ point measurements and products derived from remote sensing.

The Cosmic-Ray Neutron Sensor (CRNS) technology detects and counts naturally occurring fast neutrons (generated by cosmic-rays) after they are slowed primarily by hydrogen atoms in soil water and biomass. The CRNS can measure the root-zone SM at field-scale in a non-invasive way to an effective depth of 10 to 70 cm depending on soil water content and over a footprint of around 300 m diameter.

The AGMET group (Working Group of Applied Agricultural Meteorology in Ireland) instigated the Irish Soil Moisture Observation Network (ISMON) in 2021 and installed ten CRNS stations across Ireland, covering a range of soil types, with a view to estimating regional soil moisture conditions more accurately.

In this study, we present the SM estimates recorded since 2021 at two different ISMON sites in Ireland. In each of these sites, the CRNS sensor is co-located with arrays of Time-Domain Reflectometry (TDR) in-situ sensors. The first site is an agricultural grazing system on a mineral soil at the ISMON Farmer’s Journal farm site in Tullamore, County Offaly. The second site locates in a forest setting at the ISMON Dooray forest in County Laois. The CRNS measurements are calibrated based on soil sampling campaigns and the CRNS derived SM products are compared with TDR measurements for validation. The effect of the soil types and vegetation cover on the final SM estimates are investigated.

How to cite: Karbala Ali, H., Finkele, K., Rosolem, R., Evans, J., Schrön, M., Tobin, B., and Daly, E.: Challenges and Opportunities with Soil Moisture Measurement in Ireland using Cosmic-Ray Neutron Sensing: Examples from an agriculture and a forest site, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3236, https://doi.org/10.5194/egusphere-egu25-3236, 2025.

Lake George is a closed basin located 50 km north-east of Canberra, in southeastern Australia.  Historical records indicate that lake levels directly reflect precipitation; eight cycles of high water levels (up to 7m depth), interspersed with dry lake conditions, have occurred since 1820 CE. Over longer time scales, shoreline sediments also record phases of high water up to 14m depth in Lake George during the past 15000 years. Optically stimulated luminescence (OSL) chronologies show multiple high lake phases extending through the Holocene, with a dominant cyclic pattern of c. 2300 y.

Here we compare the Holocene lake-level data with astronomical and solar phenomena over the same time period. In particular, we calculate a cyclicity in the Grand Alignments (GAs) of the four Jovian planets of 4628 y and near GAs occurring at 2314 y intervals, the timing of which is coeval with the Lake George filling events. GAs have been observed to align with Grand Minima (GMs) (eg Maunder and Spoerer Minima) in solar activity (sunspots) which produce phases of high galactic cosmic ray flux on Earth. The timing of GMs is obtained by reconstruction of 10Be and 14C fluxes as recorded in terrestrial sediments.  These high fluxes also appear to show a temporal relationship with occurrence of the lake level highs. 

The recognition of cosmic ray flux episodes, rather than individual GMs, strongly indicates an association between observed solar activity and the high lake levels as preserved in the Lake George sediment archive. The time span 0-9.4ka contains four GM episodes and 13 OSL dated lake levels.  Of the latter, 69% date within the episodes of GM. The evidence suggests that precipitation in the Lake George basin has been associated with Jovian planet grand alignments and near GAs for at least the past 15000 years, and with phases of reduced solar and interplanetary magnetic field  strength and increased GCR flux in the vicinity of the Earth. 

The study supports the hypothesis that solar activity exhibits the well -known Hallstatt cycle periodicity (2300 yr).  Mechanisms for cause and effect remain subjects for further study.

How to cite: Asten, M., McCracken, K., and Fitzsimmons, K.: A 10ka Holocene record of cyclic precipitation in a closed catchment in SE Australia, associated with  episodes of solar Grand Minima and variations in galactic cosmic ray flux, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3395, https://doi.org/10.5194/egusphere-egu25-3395, 2025.

EGU25-3490 | ECS | Posters on site | GI4.4

Simulation of Cosmic Rays Trajectories and Neutron Transport generated on the Sun and observed on Earth 

Rocío Fuente, Carlo Luis Guerrero, Juan José Blanco, and Pablo Cerviño

The study of Cosmic Rays (CRs) and Solar Energetic Particles (SEPs) is key in analyzing the effect of solar activity on the terrestrial environment. Changes in the properties of the medium they pass through until their detection profoundly affect the intensity and the propagation direction of the CR flux.

Our starting point is that accurate measurements of CR and SEP flux can allow us to infer the conditions of the medium they pass through on their way to Earth, particularly the interplanetary medium, the magnetosphere and the atmosphere. The development of a CR simulation code helps us perform such analysis, which may contribute to future predictions of solar events and prevent potential damage and disturbances in the global technological system and the human environment. Computational simulation of these phenomena allows us to interpret the data and obtain a vision that will facilitate, for instance, explaining the generation and transport of solar neutrons to Earth’s atmosphere and their interaction with the atmosphere and the detectors installed in different geographical locations.

The Space Research Group of the University of Alcala (SGR – UAH) has extensive experience in the design, construction, control and maintenance of neutron measurement systems, distributed in different regions of the world. Among these, we can mention: CALMA, ORCA, ICaRO and the EPD aboard on the Solar Orbiter Mission. These instruments generate a large amount of data that must be analyzed and modeled for understanding and study. It is at this point where computational simulation techniques and data management are crucial for the SGR-UAH group.

In this work we present the code we developed to study the trajectory and rigidity of charged particles entering Earth’s magnetic field. The simulation code TOROS (Trajectories of cOsmic Rays Observed Simulator) is based on numerically calculating the trajectories of charged particles and their interaction with Earth’s magnetic field before reaching the atmosphere. The code uses the magnetic dipole model and various approximations of Tsyganenko’s magnetic field model. Our goal is to use this simulation tool and the data it generates as input for well known simulation codes in the research field, such as GEANT-4 and CORSIKA, to validate, simulate and propose models based on experimental measurements from detectors of the SGR-UAH group and others worldwide. Comparing our results with other simulation codes is also part of the validation and testing process for the “TOROS” code.

How to cite: Fuente, R., Guerrero, C. L., Blanco, J. J., and Cerviño, P.: Simulation of Cosmic Rays Trajectories and Neutron Transport generated on the Sun and observed on Earth, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3490, https://doi.org/10.5194/egusphere-egu25-3490, 2025.

EGU25-4551 | Orals | GI4.4

Atmospheric effect on cosmic ray produced neutron: mini neutron monitor experimental results 

Juan Jose Blanco, Du Toit Strauss, Juan Ignacio García-Tejedor, África Barreto, Pablo Cerviño-Solana, David Arrazola, Alberto Regadío, Carlo Luis Guerrero Contreras, Pablo Gonzalez-Sicilia, David Moure, Victor Cabrera, Stepan Poluianov, and Óscar García-Población

Primary cosmic rays (PCRs) interact with atmospheric nuclei producing a myriad of secondary particles known as secondary cosmic rays (SCRs) that can be measured with ground-based detectors such as neutron monitors. Neutrons, protons, pions or muons are some of the particle species of these SCRs. Their flux is related to the kinetic energy of the PCRs and shows a strong dependence on the pressure level at the observation site reflecting their dependence on the amount of matter they have to pass through the atmosphere. In addition, the air column above the observation point evolves continuously introducing temporal changes in the SCR flux due to atmospheric conditions. This atmospheric effect is taken into account by the β factor, which is the exponent of the exponential relationship between the atmospheric pressure and the SCR count rate, being mostly neutrons in the case of neutron monitors. On the other hand, pressure shows an inverse dependence with height above sea level and this should be reflected in the neutron monitor count rate as it is measured at different altitude levels. Altitude surveys with a mobile neutron monitor are essential for understanding how the atmosphere affects SCR production and for cross-checking models describing the interaction between cosmic rays and atmospheric atoms. From October 2023 to September 2024, one such survey was carried out with a mini neutron monitor on the island of Tenerife. Four sites were visited at the altitudes of 20, 868, 2390 and 3355 meters above sea level, respectively. A control point to monitor solar activity during altitude sounding has been established at the 2390 m site where a standard 3NM64 neutron monitor has been operating since early 2023 at the Izaña Atmospheric Observatory. The results of the experiment are presented and discussed and the dependence of the β factor on the multiplicity in the mini neutron monitor is noted, suggesting an energy dependence of the β factor.

How to cite: Blanco, J. J., Strauss, D. T., García-Tejedor, J. I., Barreto, Á., Cerviño-Solana, P., Arrazola, D., Regadío, A., Guerrero Contreras, C. L., Gonzalez-Sicilia, P., Moure, D., Cabrera, V., Poluianov, S., and García-Población, Ó.: Atmospheric effect on cosmic ray produced neutron: mini neutron monitor experimental results, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4551, https://doi.org/10.5194/egusphere-egu25-4551, 2025.

EGU25-5935 | Posters on site | GI4.4

Site-specific incoming correction based on muons: a comparison with cosmic neutrons measurements at JUNG at OULU. 

Carlotta Bonvicini, Gianmarco Cracco, Barbara Biasuzzi, Stefano Gianessi, Marcello Lunardon, Mario Zara, Marco Zanetti, Luca Stevanato, and Enrico Gazzola

Cosmic Rays Neutron Sensing (CRNS) opened the possibility to measure water content in the environment by neutrons absorption overcoming the need of an artificial radioactive source of neutrons. While the exploitation of a naturally available source of radiation is a fundamental feature that allows the widespread deployment of permanent sensors on-field, it intruduces the need of monitoring the natural variation of the incoming radiation to correct the signal accordingly.

This so-called “incoming correction” for CRNS is usually obtained by referring to the public data provided by the Neutron Monitor DataBase (NMDB) observatories, with the Jungfraujoch (JUNG) often being the preferred one, due to its position in central Europe on the Swiss Alps. In fact, a critical factor affecting the incoming flux of cosmic rays at the ground is the geomagnetic cutoff rigidity parameter, which is site-specific with a strong dependence on the latitude. The site-specificity of the incoming correction, together with the need to rely on an external source of data, makes it a crucial topic for the CRNS community.

Finapp developed a patented detection technology with the feature of contextually detecting neutrons and muons. Muons are also generated by cosmic rays, but they are not backscattered by the soil like neutrons, which makes them suitable for monitoring the incoming flux itself. In order to provide a fair, site-specific comparison between the variations of muons counts by Finapp and cosmic neutrons counts by NMDB observatories, we installed a sensor at the NMDB-JUNG site in January 2024 and one at the NMDB-OULU site in Finland in October 2024. In this presentation we will report preliminary results of this project and its impact on CRNS applications.

We acknowledge the NMDB database (www.nmdb.eu), founded under the European Union's FP7 programme (contract no. 213007) for providing data. Jungfraujoch neutron monitor data were kindly provided by the Physikalisches Institut, University of Bern, Switzerland. Oulu neutron monitor data were kindly provided by the Sodankyla Geophysical Observatory (https://cosmicrays.oulu.fi).

How to cite: Bonvicini, C., Cracco, G., Biasuzzi, B., Gianessi, S., Lunardon, M., Zara, M., Zanetti, M., Stevanato, L., and Gazzola, E.: Site-specific incoming correction based on muons: a comparison with cosmic neutrons measurements at JUNG at OULU., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5935, https://doi.org/10.5194/egusphere-egu25-5935, 2025.

EGU25-6803 | ECS | Posters on site | GI4.4

A worst-case scenario? Exploring low-energy cosmic-ray neutron signal dynamics in wetlands 

Daniel Rasche, Torsten Sachs, Aram Kalhori, Christian Wille, Markus Morgner, Andreas Güntner, and Theresa Blume

In the past 15 years, Cosmic-Ray Neutron Sensing (CRNS) has evolved to a useful tool for monitoring soil moisture at the field scale. Given the large measurement radius of up to 200 metres and measurement depth of 20 to 30 centimetres, it overcomes small-scale heterogeneities and allows to estimate soil moisture at spatio-temporal scales which are required to e.g., inform environmental models or validate soil moisture products from remote sensing data.

CRNS relies on the inverse relationship between soil moisture and observed low-energy cosmic-ray neutrons. Higher soil moisture results in lower neutron intensities but also a higher statistical noise in the data. In combination with the strongly non-linear relationship between soil moisture and observed low-energy cosmic-ray neutrons, this leads to larger uncertainties for soil moisture estimates when the soil moisture is high. Therefore, CRNS is expected to provide most accurate soil moisture estimates at monitoring sites with generally drier soils. Knowledge gaps remain with respect to the use of CRNS and the response of measured neutron intensities at observation sites with very wet soils and even partial water cover.

Against this background, we explore the signal dynamics of observed thermal and epithermal neutron intensities in a wetland in north-eastern Germany. Placing two identical neutron detectors at two different locations in the wetland and with different fractions of water cover in their respective measurement footprint allows for an investigation of the sensitivity of observed neutron signals to variations in partial water cover and soil moisture changes in water-free areas. Site-specific signal dynamics are modelled using neutron transport simulations conducted with the URANOS model code as well as simplified approaches to gain understanding on the influence of water cover and soil moisture on thermal and epithermal neutron signals. Ultimately, the possibility of deriving soil moisture information in water-free areas from observed neutron intensities is explored.

Our analyses shed additional light on the potential of CRNS for soil moisture estimation and its sensitive measurement footprint at extreme and unfavourable monitoring sites.

How to cite: Rasche, D., Sachs, T., Kalhori, A., Wille, C., Morgner, M., Güntner, A., and Blume, T.: A worst-case scenario? Exploring low-energy cosmic-ray neutron signal dynamics in wetlands, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6803, https://doi.org/10.5194/egusphere-egu25-6803, 2025.

EGU25-8780 | ECS | Posters on site | GI4.4

The additive value of multi-scale remote sensing snow products for alpine above-snow Cosmic Ray Neutron Sensing 

Nora Krebs, Paul Schattan, Valentina Premier, Abraham Mejia-Aguilar, Christine Fey, Magnus Bremer, and Martin Rutzinger

Alpine snow cover is shaped by complex topography, wind and insulation patterns, causing strong lateral heterogeneity in snow water equivalent (SWE) within only a few meters distance. While common SWE observation methods are confined to a footprint area of a few square meters, above-snow cosmic ray neutron sensing (CRNS) detects secondary cosmogenic neutrons that can be translated to SWE from an area of several hectares. The large footprint size decreases the observation bias that is caused by the choice of measurement location in conventional methods. However, the large footprint size also decreases the control on other signal contributing factors. Cosmogenic neutrons are sensitive to all sources of ambient hydrogen, including soil moisture and vegetation. Partial snow cover poses an additional challenge, due to the dissimilar and non-linear contribution of snow-free and snow-covered areas. The predominant development of mountain snowpack into partial snow cover highlights the intricacy of the CRNS signal in the alpine domain. In this study, we explore the complementary value of close-range, mid-range and far-range remote sensing snow products for the characterization of alpine CRNS snow monitoring sites in Austria and Italy. Joined observations of satellite-based fractional snow cover (FSC) products of Sentinel-1 and -2 and MODIS, at a spatial resolution of 20 m, 60 m and 500 m, respectively, provide quasi-daily observations of the snow cover state within the CRNS footprint area. This allows us to identify site-specific snow season parameters and dynamics in the CRNS signal. Further, air-borne and terrestrial topographic lidar (ALS and TLS) campaigns under snow-free and snow-covered conditions provide detailed FCS, snow height distribution and topographic information at a high spatial resolution. The good compatibility of these products is shown by the overall low deviation between lidar derived FSC and Sentinel FSC products of ~11% and between lidar and MODIS FSC of ~13%. Paired with complementary, manual snow density measurements for the computation of distributed SWE and the calibration of the neutron count to SWE conversion, these observations allow us to evaluate the complexity and dynamics of the seasonal CRNS signal at alpine sites. The similarity in spatial resolution between CRNS and satellite-based remote sensing products points towards its high potential for bridging the gap between ground- and space-based snow observations. Dedicated neutron simulations and further investigations are needed to gain a better understanding of factors that contribute to neutron count dynamics in alpine terrain.

How to cite: Krebs, N., Schattan, P., Premier, V., Mejia-Aguilar, A., Fey, C., Bremer, M., and Rutzinger, M.: The additive value of multi-scale remote sensing snow products for alpine above-snow Cosmic Ray Neutron Sensing, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8780, https://doi.org/10.5194/egusphere-egu25-8780, 2025.

Secondary cosmic rays (CRs) are produced when primary CRs interact with atmospheric atoms, leading 
to the formation of a cascade of secondary particles such as neutrons, pions, protons, and muons, with 
energies ranging from a few dozen meV to over 1 GeV. Neutrons produced during the extensive air 
shower spreading is characterized by a high elastic scattering cross section with hydrogen nuclei. This 
latter effectively moderates neutrons by slowing them down, and composes different media in the 
atmosphere, such as water vapor, ice and liquid vapor. 
Neutron spectrometry is based on this singular ability of hydrogen to moderate neutrons. In addition of 
interacting with the atmosphere, cosmic neutrons also interact with the Earth’s surface. Some of them 
are scattered back to the surface and are referred to as albedo neutrons. This phenomenon is crucial for 
studying soil moisture with a Bonner sphere spectrometer. Indeed, previous studies on both neutrons 
monitors and Bonner spheres spectrometers highlighted the impact of soil water content on neutron fluxes, 
validating the use of these methods to monitor soil moisture. However, it has been established that 
atmospheric water vapor induces a significant decrease in neutron counts that requires consideration. 
For this study, an experimental platform was deployed at the Atmospheric Research Center in 
Lannemezan, France. This platform includes instruments monitoring the atmospheric column 
hygrometry (precipitations, mixing ratio) and pressure -provided by a 60 m high mast- and soil moisture 
variations measured by refractometric probes in a 120 cm depth pit. In addition, a BSS extended to high 
neutron energies is constantly measuring the neutronic natural environment near the pit and mast since 
September 2023. The Bonner sphere spectrometer consists of three high-density polyethylene spheres 
(3, 5, and 8 inches) and two polyethylene spheres with inner high-density metal shells (8 and 9 inches), 
each equipped with a 2-inch proportional counter. This instrument provides a valuable information about 
the detected neutrons by allowing the reconstruction of the full spectrum, from meV to GeV. Thus, this 
approach enables the study of the impact of different hydrogen pools across the four main energy 
domains (thermal, epithermal, evaporation, and cascade neutrons). 
To complement these experimental data, a simulation work was necessary. The URANOS (Ultra Rapid 
Neutron Only Simulation) code has been a reference for several years in the field of simulating the 
transport of atmospheric neutrons in the atmosphere and soils. It is based on the application of the Monte 
Carlo method, and allows to calculate physical quantities such as energy distribution, spatial distribution, 
and neutron interaction processes. To meet more accurately the needs of this study, a module 
specifically designed for Bonner Spheres has been developed, providing key information on the impact 
of the atmosphere on neutron counts measured by each sphere.  
In this study, we apply a new methodology to a set of experimental time series in order to reduce the 
impact of the atmosphere on neutron counts from the Bonner sphere spectrometer. We will finally 
compare the results to the same uncorrected time series. 

How to cite: Tilhac, A., Hubert, G., Köhli, M., and Lohou, F.: Improving neutron spectrometry measurement methodology to better understand soil moisture variability: application to an area subject to strong seasonal and daily variations , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11397, https://doi.org/10.5194/egusphere-egu25-11397, 2025.

EGU25-11935 | ECS | Posters on site | GI4.4

Adverse conditions for cosmic-ray neutron sensing: high water content low bulk density – can we still infer soil moisture over the full moisture range? 

Peter Grosse, Lena Scheiffele, Sophia Dobkowitz, Katya Dimitrova-Petrova, Daniel Rasche, and Sascha Oswald

Near-surface soil moisture variation is an important variable in peatlands, controlling chemical processes and peat development or degradation. Cosmic-ray neutron sensing (CRNS) provides an area average soil moisture over a support volume of > 150 m radius and down to 50 cm depth by relating the abundance of secondary fast neutrons above ground to soil moisture. However, standard calibration and weighting functions for CRNS were developed and tested for mineral soils with dry bulk densities above 1 g cm-³ and only up to 55 % of volumetric soil moisture. Peat soils, in contrast, are characterized by high organic matter content, low bulk densities, and high soil moisture when saturated. This makes peatlands a challenging environment for any soil moisture monitoring, including CRNS. In such adverse conditions, questions remain on the appropriate CRNS calibration approach and therefore the accurate determination of soil moisture.

This study presents lessons learned from operating a CRNS at a fen site with extensively used grassland in Northeast Germany (nature conservation area “Kremmener Luch”) for 3.5 years. The CRNS was complemented with point-scale soil moisture sensor profiles down to 1 m (FDR and TDR) in several locations of its footprint as well as groundwater level observations to identify periods of ponding that occur frequently at the site. Measuring soil moisture with the dielectric point-scale sensors showed challenges on its own. We increased the precision of point-scale data by a local soil specific calibration relating sensor permittivity to soil moisture. However, strong jumps and unreliable values remained, presumably due to swelling and shrinking of the organic-rich soil and loss of contact with the sensor. FDR and TDR time series showed large differences in absolute values as well as spatially different soil moisture regimes due do effects of microtopography. This is opposed to the CRNS, which senses average water content independent of small-scale heterogeneities. To derive a CRNS soil moisture time series we tested calibrating the CRNS using data from dedicated soil moisture sampling campaigns or the point-scale time series. We obtained unrealistically high CRNS-soil moisture regardless of which calibration function we chose – the standard “Desilets’ equation” or the recently proposed advanced “Universal Transport Solution”. Following the suggestion in previous CRNS studies conducted at peaty sites, we adjusted the parameters of the Desilets’ equation, which lead to a more realistic soil moisture range. However, the estimation of the CRNS integration depth with the standard procedures is very sensitive to the low bulk density of the organic soil and remains largely uncertain. This data set serves as a valuable testbed for extending the validity of existing calibration and weighting functions, and we will utilize neutron simulations to enhance our understanding of the vertical footprint of CRNS under conditions of low bulk density and high soil moisture.

Improved understanding and precision of CRNS soil moisture in peatlands can support peatland restoration efforts by providing insights into near-surface soil moisture variations allowing the evaluation of water level management success.

How to cite: Grosse, P., Scheiffele, L., Dobkowitz, S., Dimitrova-Petrova, K., Rasche, D., and Oswald, S.: Adverse conditions for cosmic-ray neutron sensing: high water content low bulk density – can we still infer soil moisture over the full moisture range?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11935, https://doi.org/10.5194/egusphere-egu25-11935, 2025.

EGU25-12050 | ECS | Orals | GI4.4

The Role of Aerosol Types in Mediating the Impact of Galactic Cosmic Rays on Climate Variability Over the Past Two Decades 

Faezeh Karimian Sarakhs, Fabio Madonna, and Salvatore De Pasquale

Galactic Cosmic Rays (GCRs), high-energy particles originating from supernovas, have been hypothesized to influence Earth's climate by ionizing atmospheric aerosols and accelerating the formation of cloud condensation nuclei (CCN). This mechanism leads to increasing the cloud cover and enhances the cooling effect at the Earth’s surface. However, the magnitude of this natural forcing remains a subject of debate. This study proposes the use of multivariate linear regression to model monthly anomalies in near-surface air temperatures as a function of anomalies in GCR flux and other solar and climate variables, including sunspot number, geomagnetic indices, greenhouse gas concentrations (CO₂ and CH₄), cloud effective radius (CER), cloud liquid water, radiation, and aerosol optical depth (AOD) across different latitudes. Monthly data  collected over the past 20 years from a variety of instruments, surface-based and satellite on board, and networks monitoring the atmosphere and from three neutron monitoring stations at different latitudes:  in Hermanus (South Africa, low-latitude), Newark (USA, mid-latitude), and Oulu (Finland, high-latitude) have been considered, being the location of three neutron monitor stations. CER and AOD emerged as the most significant predictors across all stations. Incorporating GCR flux as a covariate for AOD improved model performance, with adjusted R-squared values increasing from 0.22 to 0.31 in Oulu, 0.37 to 0.52 in Newark, and 0.69 to 0.78 in Hermanus. Further analysis using ECMWF atmospheric composition reanalysis indicated that sea salt aerosols, particularly in the 5–20 µm size range, dominate across all locations, suggesting their potential role to the mechanisms enhanced by the GCRs ionization power, such as CCN formation and particle aggregation. A next step would be to investigate the impact of GCRs on cloud characteristics, such as cloud cover, cloud fraction and cloud top properties like pressure and temperature, to gain a clearer understanding of their influence on climate variability.

Keywords: galactic cosmic ray, near surface temperature, aerosol type, sea salt aerosol, cloud condensation nuclei, climate natural variability

How to cite: Karimian Sarakhs, F., Madonna, F., and De Pasquale, S.: The Role of Aerosol Types in Mediating the Impact of Galactic Cosmic Rays on Climate Variability Over the Past Two Decades, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12050, https://doi.org/10.5194/egusphere-egu25-12050, 2025.

EGU25-12351 | Posters on site | GI4.4

Irrigation Management and Soil Moisture Monitoring with Cosmic-Ray Neutron Sensors: Lessons Learned and Future Opportunities 

Heye Bogena, Cosimo Brogi, Felix Nieberding, Andre Daccache, Lena Scheiffele, and Salar Saeed Dogar

Cosmic Ray Neutron Sensing (CRNS) is attracting attention in irrigation management. CRNS can non-invasively and accurately measure soil moisture (SM) in the root zone at the field scale, thus addressing scale and logistics issues typical of point-scale sensor networks. CRNS are effectively used to inform large pivot irrigation systems but most agricultural landscapes in Europe and elsewhere consist of highly diversified and small fields. These are challenging for CRNS as the measured signal integrates an area of ~200m radius where multiple fields, soil heterogeneities, or variable amount of water applications can be found.

In this work, we present results from three case studies, and we develop and test solutions to improve CRNS accuracy in irrigated contexts. In 2023, a potato field in Leerodt (Germany) where strip irrigation is practiced was equipped with three CRNS (with moderators and thermal shielding), three meteorological stations, and six profile SM probes measuring at six different depths (up to 60 cm). In the same year, in Davis (California, USA), two CRNS with a 15 mm moderator, one of which also had a thermal shielding, were installed in an alfalfa field where flood irrigation is practiced. These were supported by meteorological measurements and point-scale TDR sensors. Similarly, a CRNS installed in a winter wheat field in Oehna (Germany) where pivot irrigation is applied. As the origin and propagation of neutrons detected by a CRNS cannot be inferred from the measured signal, we used the URANOS model to analyze neutron transport in the three case studies under varying soil moisture scenarios. To account for soil heterogeneity in the Leerodt study, we assessed the spatial distribution of soil characteristics by integrating soil sampling and Electromagnetic Induction (EMI) measurements in a machine-learning framework.

The Leerodt study showed that CRNS outperformed point-scale sensors, which were strongly affected by soil erosion in the top 10 cm. However, CRNS was unexpectedly sensitive only to nearby irrigation. Here, key insights on sub-footprint heterogeneity and soil roughness were gained through the analysis of URANOS simulations. In the Davis study, CRNS effectively monitored irrigation but also showed unexpected sensitivities to the irrigation of distant fields. Again, important insights were gained thanks to URANOS simulations. In the Oehna study, large quantitative differences between the CRNS and point-scale sensors were observed. However, the CRNS provided clear responses to irrigation that can outperform the information provided by the point-scale devices. Overall, the limitations of CRNS-based irrigation management in complex agricultural environments can generally be overcome through a synergetic use of measurements and modelling. Nonetheless, more efforts are needed to improve the understanding of the underlying processes and to standardize measurement procedures, which ultimately requires the involvement not only of researchers but also of manufacturers and stakeholders.

How to cite: Bogena, H., Brogi, C., Nieberding, F., Daccache, A., Scheiffele, L., and Dogar, S. S.: Irrigation Management and Soil Moisture Monitoring with Cosmic-Ray Neutron Sensors: Lessons Learned and Future Opportunities, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12351, https://doi.org/10.5194/egusphere-egu25-12351, 2025.

EGU25-12782 | ECS | Orals | GI4.4

On the use of geophysics to support and connect soil sensors and cosmic ray neutron sensing: a case study highlighting the relevance of soil heterogeneity 

Luca Peruzzo, Mirko Pavoni, Viola Cioffi, Matteo Censini, Francesca Manca, Ilaria Barone, Matteo Verdone, Jacopo Boaga, and Giorgio Cassiani

Precision agriculture directly points at both spatial and temporal variabilities, to be mapped and monitored with relevant technologies. With regard to the subsurface, soil sensors remain the foremost driver of precision agriculture. These sensors provide high temporal resolution information on key soil variables, including volumetric water content. However, their limited representativeness and high sensitivity to local and installation factors are intrinsic and well known issues. Cosmic ray neutron sensing (CRNS) is a newer technology that addresses these issues, with the water content information being integrated over a footprint of several tens of meters. Nonetheless, the integrated water information remains a one-dimensional time series. The interplay of different spatial scales of the measurements and unknown subsurface heterogeneity ultimately hinders the correct interpretation of the individual time series, and their discrepancies.

In this work we explore how geophysics-based soil heterogeneity supports the interpretation of time series from soil water sensors and cosmic ray neutron sensing. We present a case study from a vineyard in the Chianti region (Siena, Italy). We focus on the joint use of electrical resistivity tomography and frequency-domain electromagnetic induction. Two field campaigns, conducted in April and November 2024, highlight significant differences in both soil composition (clay content) and soil depth over the vineyard. Before the geophysical campaign, the soil water sensors were installed in a region with particularly deep and clayey soil. On the contrary, the cosmic ray was installed at the center of the vineyard and thus responds to regions with dominant water dynamics. The results show that the differences in water dynamics between the clay-rich area (with the soil sensors) and the surrounding areas coupled with the larger CRNS sensitivity to faster-draining regions lead to significant discrepancies. The geophysics-based spatial information qualitatively explains these discrepancies and supports CRNS numerical simulations (Uranos) that aim to provide a more quantitative understanding.

How to cite: Peruzzo, L., Pavoni, M., Cioffi, V., Censini, M., Manca, F., Barone, I., Verdone, M., Boaga, J., and Cassiani, G.: On the use of geophysics to support and connect soil sensors and cosmic ray neutron sensing: a case study highlighting the relevance of soil heterogeneity, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12782, https://doi.org/10.5194/egusphere-egu25-12782, 2025.

Evaluating the effects of galactic cosmic rays (GCR) and space weather throughout the atmosphere has motivated development of new instruments. A 1 x 1 x 0.8 cm3 and 30g microscintillator detector was flown on a meteorological radiosonde over the UK, reaching an altitude of 32 km. The flight was intended as a technology demonstrator for an improved version of the microscintillator that interfaces with the industry standard Vaisala RS41 radiosonde. GCR neutrons are regularly measured at the surface and assumed to be an indicator of ionisation above. However, neutrons are not ionising, and there are known discrepancies between surface neutrons and ionising radiation aloft. Our microscintillator is sensitive to ionising radiation with energies from 25keV-10MeV. Each pulse is recorded and pre-processed on the balloon into 17 energy channels for real-time radio transmission to a ground station.

The flight, on the afternoon of 9th July 2024, occurred during minimal solar and space weather activity, therefore the measurements are almost entirely from the cosmic ray background. The system also recorded count rates from two Geiger counters, both independently and as “coincidences” from simultaneous triggering from higher energy particles. As anticipated, the background count rate in the microscintillator and Geigers increased as the balloon ascended, reaching the Regener-Pfotzer maximum, in this case at 22 km. Peaks in the energy spectrum occurred at 1.8 MeV, likely to be due to the gamma rays produced through de-excitation of atmospheric nitrogen nuclei excited by secondary GCR neutrons. Detection of gamma rays from neutron interactions offers the possibility of a direct comparison to neutron monitors. There were also peaks at 300keV which may be from secondary electrons created by GCR. Unlike previous flights of this detector during space weather activity, no bremsstrahlung X rays at ~100keV were observed. The Geiger and coincidence counter results were consistent with the medium and high- energy channels from the microscintillator, respectively. This combination of altitude and energy resolution is highly unusual for such a small and light weight detector.

How to cite: Aplin, K. and Tabbett, J.: Cosmic ray energy spectrum in the atmosphere measured with a novel balloon-carried detector, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13265, https://doi.org/10.5194/egusphere-egu25-13265, 2025.

EGU25-13563 | Orals | GI4.4

Observation of the Forbush decrease during the May 2024 solar storms with different muon and neutron detectors in the high-latitude site of the Svalbard archipelago 

Ombretta Pinazza, Lasse Hertle, Francesco Riggi, and Martin Schrön and the EEE Collaboration

During the series of intense solar flares that occurred in May 2024, a remarkable Forbush decrease in the cosmic ray flux was observed on the Earth by particle detectors around the world. The Svalbard archipelago, which is located at polar latitudes, is particularly exposed to geomagnetic storms because the Earth's magnetic field provides a particularly weak shielding and is therefore a privileged observation point. In this contribution, we report an analysis of the Forbush decrease event using data from a unique combination of muon and neutron detectors installed in Ny-Ålesund, on Svalbard: three scintillator-based muon telescopes of the Extreme Energy Events (EEE) Project, 14 channels of a Bonner Sphere neutron Spectrometer (BSS), thermal and epithermal neutron sensors used for hydrological monitoring, and a high-energy neutron monitor located in Barentsburg and operated by the Polar Geophysical Institute. We found that most sensors showed significant responses and correlation during the event. The observed magnitude of the Forbush decrease depended on the detector’s energy sensitivity and was 10% for thermal neutrons, 8% for high-energy neutrons, and 3% for muons. The uncertainty of these results strongly depends on factors like the count rate, which ranged from 10 to 105 cph and resulted in low signal-to-noise ratio, particularly for the BSS. A detailed correlation analysis was carried out among the various time series originated from the different detectors in the “quiet” period (before the Forbush decrease) and during the Forbush event. Multi-particle and multi-energy observations provide an unprecedented view on the Earth’s exposure to cosmic rays during solar events.

How to cite: Pinazza, O., Hertle, L., Riggi, F., and Schrön, M. and the EEE Collaboration: Observation of the Forbush decrease during the May 2024 solar storms with different muon and neutron detectors in the high-latitude site of the Svalbard archipelago, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13563, https://doi.org/10.5194/egusphere-egu25-13563, 2025.

EGU25-15027 | Orals | GI4.4

Scaling Cosmic Ray Neutron Flux for Enhanced Environmental Monitoring 

Roland Baatz, Patrick Davies, Paolo Nasta, Paul Schattan, Emmanuel Quansah, Leonard Amekudzi, and Heye Bogena

Cosmic Ray Neutron Sensors (CRNS) are pivotal in measuring field-scale soil moisture, but uncertainties persist due to traditional methods of scaling parameter estimation, which often fail to consider site- and sensor-specific factors. This study integrates novel, data-driven approaches to refine scaling parameters for atmospheric pressure, air humidity and incoming cosmic ray intensity (β, ψ, ω) using measurement data. We demonstrate the strong potential for considerable improvents in the accuracy of CRNS-derived soil moisture estimates. Additionally, barometric correction in CRNS but also in neutron monitors is critical to account for local atmospheric density variations to minimize errors in soil moisture estimation and incoming cosmic ray intensity. Our analysis of CRNS and Neutron Monitor data from global stations reveals significant variability in barometric coefficients (β), influenced by geographical and atmospheric factors. The findings underscore the necessity for tailored scaling and correction methods to optimize CRNS applications in hydrology, agriculture, and climate research. Enhanced parameter estimation reduced RMSE by up to 25%, demonstrating potential for improved environmental decision-making and modeling accuracy.

How to cite: Baatz, R., Davies, P., Nasta, P., Schattan, P., Quansah, E., Amekudzi, L., and Bogena, H.: Scaling Cosmic Ray Neutron Flux for Enhanced Environmental Monitoring, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15027, https://doi.org/10.5194/egusphere-egu25-15027, 2025.

EGU25-15979 | Orals | GI4.4

Validation of rail based CRNS-roving: underpinning the large-scale root zone soil moisture monitoring concept 

Daniel Altdorff, Solveig Landmark, Merlin Schiel, Sascha E. Oswald, Steffen Zacharias, Peter Dietrich, Hannes Mollenhauer, Sabine Attinger, and Martin Schrön

Root zone soil moisture (RZSM) is a critical parameter for various environmental, agricultural, and hydrological applications. The recently proposed rail based Cosmic Ray Neutron Sensing monitoring method (Rail-CRNS) offers an innovative solution for soil moisture measurement by enabling continuous, large-scale RZSM measurements across extensive railway networks. By 2024, Germany established a fleet of five Rail-CRNS systems, covering up to hundreds of kilometers daily and marking thus a transformative step in soil moisture monitoring. Yet, questions remained regarding the reliability of Rail-CRNS data: did they accurately capture RZSM, or were they overly influenced by confounding factors such as land use and rail track conditions?

This study addresses these questions by analyzing 16 months of Rail-CRNS data collected along a pilot route in Rübeland, Low Harz Mountain, Germany. Time series from two stationary CRNS sites, located in forested and grassland areas, were compared with corresponding Rail-CRNS data segments. Additionally, soil moisture measurements from buried sensor nodes in the forest provided for parts of the period another independent reference dataset. The results demonstrated a strong correlation between the stationary CRNS measurements, the Rail-CRNS-derived RZSM values, and the soil moisture node data. This alignment indicates that Rail-CRNS data reliably captures not only spatial but also temporal variability in soil moisture. These findings provide robust support for the Rail-CRNS concept, emphasizing its potential to generate accurate and high-resolution RZSM data for regional and national-scale monitoring.

However, the pilot study was conducted under specific and well-monitored conditions, with frequent train passages and a well-instrumented route. Applying the Rail-CRNS method to longer, less-instrumented tracks, combined with higher train speed variability and fewer repeated passes, will likely introduce greater uncertainties. To address this, the deployment of a CRNS station cluster near railways was proposed. Such clusters would enable ongoing validation of Rail-CRNS data, ensuring their reliability across diverse environmental and operational conditions.

This study underscored the transformative potential of Rail-CRNS in overcoming the long-standing challenges of sparse and incomplete RZSM measurements. However, further instrumentation and research is planned to develop strategies for mitigating potential uncertainties in less-controlled environments. Integrating Rail-CRNS data with satellite-based products and RZSM estimates from hydrological modeling for example could further enhance the accuracy and applicability of soil moisture monitoring on a national scale.

How to cite: Altdorff, D., Landmark, S., Schiel, M., Oswald, S. E., Zacharias, S., Dietrich, P., Mollenhauer, H., Attinger, S., and Schrön, M.: Validation of rail based CRNS-roving: underpinning the large-scale root zone soil moisture monitoring concept, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15979, https://doi.org/10.5194/egusphere-egu25-15979, 2025.

EGU25-17007 | ECS | Posters on site | GI4.4

A Gamma Ray and Neutron Spectrometer (GRNS) for mapping lunar surface composition and water abundance on the SER3NE mission 

Rebecka Wahlén, Ramsey Al Jebali, Luis Teodoro, and Anja Kohfeldt

Selene’s Explorer for Roughness, Regolith, Resources, Neutrons and Elements (SER3NE) is a lunar orbiter mission designed to map the topmost composition of the lunar surface, including elemental composition and water abundance. Planned instruments include a Gamma Ray and Neutron Spectrometer (GRNS) for elemental composition, including hydrogen indicating water, a Laser Altimeter (LA) for surface roughness and albedo observations, and a near-infrared spectrometer (LIPS) to determine water forms.

The GRNS detector is designed for both in situ utilization as well as remote sensing. It has a core of CLLBC and LaBr3 crystal scintillators in a chessboard pattern for high-resolution gamma-ray detection (30 keV-8MeV) and thermal to epithermal neutron sensitivity. Gd foil on CLLBC allows separation of thermal and epithermal neutrons, while LaB3 and CLLBC enable advanced neutron detection analysis. Encapsulated by EJ-248M plastic scintillators, the detector includes anti-coincidence detector for charged particle rejection. With gamma-ray spectroscopy, rock-forming elements as well as KREEP and trace elements can be detected in the shallow surface of the moon. The local count rates of thermal and epithermal neutrons allow for the analysis of the distribution of hydrogen on the lunar surface, as well as for estimation of neutron lifetime from the lunar orbit.

A demonstrator of the GRNS instrument has been successfully tested in the lab. A prototype of this lunar GRNS instrument will fly on the CENSSat-1 Bifrost CubeSat mission, scheduled for launch 2027.

In this presentation, the GRNS instrument concept will be presented, focusing on the detector design and suitability for elemental composition analysis on a lunar orbiter.

How to cite: Wahlén, R., Al Jebali, R., Teodoro, L., and Kohfeldt, A.: A Gamma Ray and Neutron Spectrometer (GRNS) for mapping lunar surface composition and water abundance on the SER3NE mission, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17007, https://doi.org/10.5194/egusphere-egu25-17007, 2025.

EGU25-17136 | ECS | Orals | GI4.4

Bonner Sphere Spectrometer at the Environmental Research Station Schneefernerhaus: Measuring Cosmic Radiation and Facilitating Data Accessibility 

Jonas Marach, Thorsten Klages, Vladimir Mares, Marcel Reginatto, Till Rehm, Werner Rühm, and Miroslav Zboril

In 2024, Germany’s national metrology institute, the Physikalisch-Technischne Bundesanstalt (PTB), signed a sponsorship agreement with the Operational Company of the Environmental Research Station Schneefernerhaus (Umweltforschungsstation, UFS) for the operation, maintenance and upgrade of the Bonner sphere-based neutron spectrometer located at the UFS. The UFS Schneefernerhaus was established in 1999 and is Germany’s highest research station at an altitude of 2650 meters, just below the summit of Mt. Zugspitze, where it houses a wide range of scientific instruments for observing weather, climate and climate change.

The Bonner Sphere Spectrometer (BSS) system at the UFS Schneefernerhaus has been in operation since 2005, thanks to the cooperation between the UFS Operational Company and the German Research Center for Environmental Health of the Helmholtz Center Munich. The system is used for continuous measurements of the neutron component of secondary cosmic radiation. With an extensive set of polyethylene sphere moderators and spheres with metal shells, the BSS at Schneefernerhaus can detect neutrons with energies ranging from 10-9 MeV to 103 MeV. Thanks to its spectrometric capabilities, the system can provide neutron energy spectra, which is an advantage over the classical neutron monitors used worldwide.

The Neutron Radiation Department of PTB is currently working on upgrading the data acquisition hardware and software, data storage, workflow and data analysis of the BSS system towards an automated and robust operation.

This presentation introduces methods for error correction and data preparation, incorporating historical data (years 2013 to 2024) from the former team of the Helmholtz Center Munich, and discusses possibilities for disseminating the data to scientific communities.

How to cite: Marach, J., Klages, T., Mares, V., Reginatto, M., Rehm, T., Rühm, W., and Zboril, M.: Bonner Sphere Spectrometer at the Environmental Research Station Schneefernerhaus: Measuring Cosmic Radiation and Facilitating Data Accessibility, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17136, https://doi.org/10.5194/egusphere-egu25-17136, 2025.

EGU25-18234 | ECS | Posters on site | GI4.4

neptoon: An extensible software package for processing CRNS data 

Daniel Power, Steffen Zacharias, Fredo Erxleben, Rafael Rosolem, and Martin Schrön

The increasing adoption of Cosmic-Ray Neutron Sensors (CRNS), across research infrastructures and beyond, necessitates standardised and flexible processing tools. Such tools should be accessible to new users with little experience in CRNS, as well as support researchers investigating novel processing methodologies and developing new theoretical frameworks. Here we present neptoon; an open-source python tool, using a modular, expandable framework, to ensure long term viability and software sustainability. Building from previous CRNS processing tools, we will present the overall architecture of neptoon and how it implements established processing methodologies while maintaining extensibility for emerging approaches. We will demonstrate streamlined data processing workflows through our configuration system and graphical user interface. We will show how neptoon supports replicability when processing sensors, supporting rapid updates when needed. Furthermore, we will showcase how neptoon enables systematic testing of new processing theories for CRNS, such as alternative correction methods, leading to a software that supports both operational deployment and methodological research. Lastly we will outline our roadmap for neptoon, explaining features which will be implemented in the near future. By creating a fully documented software toolset for processing, we aim to support the growing community of CRNS users and researchers.

How to cite: Power, D., Zacharias, S., Erxleben, F., Rosolem, R., and Schrön, M.: neptoon: An extensible software package for processing CRNS data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18234, https://doi.org/10.5194/egusphere-egu25-18234, 2025.

EGU25-18374 | Posters on site | GI4.4

Approaches and Challenges of the Neutron Monitor based Incoming Flux Correction for Cosmic-Ray Neutron Sensing 

Lasse Hertle, Steffen Zacharias, Nicholas Larsen, Daniel Rasche, and Martin Schrön

Cosmic Ray Neutron Sensing (CRNS) is a technique to measure water content, for example soil moisture, on the hectare scale through the measurement of epithermal neutrons. The neutrons are results of  particle showers in the earth's atmosphere caused by cosmic rays impinging on it. The abundance and global distribution of neutrons is changed in time through different factors. On the largest scale, the heliosphere and therefore the solar cycle greatly affect the amount of galactic cosmic rays that are able to reach earth. Large solar events, such as Forbush decreases, also cause rapid changes in the cosmic ray flux. The aim of any incoming neutron flux correction method is ultimately to account for these heliospheric changes. Any neutron monitor based correction method has to overcome the uneven distribution of neutrons across latitudes, due to the earth's magnetic field.  There have been multiple, neutron monitor based, approaches developed, all of them based upon the assumption of linearity between the CRNS and the neutron monitor measurement. This assumption is challenged by multiple factors, most importantly geomagnetic and local conditions. Understanding the challenges and limitations of the linearity assumption is crucial to reliably correct CRNS measurements and produce a robust soil moisture product. Multiple correction methods have been evaluated and compared, with consideration towards the impact of different geomagnetic and local conditions. 

How to cite: Hertle, L., Zacharias, S., Larsen, N., Rasche, D., and Schrön, M.: Approaches and Challenges of the Neutron Monitor based Incoming Flux Correction for Cosmic-Ray Neutron Sensing, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18374, https://doi.org/10.5194/egusphere-egu25-18374, 2025.

EGU25-19126 | ECS | Posters on site | GI4.4

Reduced ERA-I forecasting skill during Forbush decreases 

Jacob Svensmark

Previously, week-long Forbush decreases of the atmospheric cosmic ray flux have been found to correlate with terrestrial cloud cover changes. Discussions are ongoing on whether this correlation is caused by a physical mechanism or simply a result of unlikely weather fluctuations. To gain further insight on this matter, we consider the skill of weather forecasts during Forbush decreases using data from the ERA-INTERIM forecasting system. If the cloud changes during Forbush decreases are of meteorological origin, then they should be forecasted by ERA-INTERIM at a skill comparable to any other time. On the contrary, if the cosmic ray flux is coupled to clouds, forecasts should be performing worse during Forbush decreases, since ERA-interim is insensitive to cosmic rays. We find, that ERA-INTERIM was significantly worse at predicting the total cloud cover in times of large Forbush decreases compared to outside of them, supporting the hypothesis that cosmic rays influence terrestrial cloud formation.

How to cite: Svensmark, J.: Reduced ERA-I forecasting skill during Forbush decreases, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19126, https://doi.org/10.5194/egusphere-egu25-19126, 2025.

EGU25-19534 | ECS | Posters on site | GI4.4

Mars Radiation Environment and Water-ice Prospecting through a Distributed Swarm of Tumbleweed Rovers  

Mário de Pinto Balsemão, Abhimanyu Shanbhag, James Kingsnorth, Gergana Bounova, Luka Pikulić, Cristina Moisuc, Daan Molhuijsen, and Julian Rothenbuchner

The Tumbleweed mission aims to revolutionize Mars exploration by leveraging the unique capabilities of wind-driven, spheroidal rovers. The use of modular design strategies, off-the-shelf components, and mass production will significantly reduce costs, making Mars exploration more accessible. Designed for rapid and extensive surface exploration, Tumbleweed rovers offer an affordable and efficient method for gathering crucial data across large areas of the Martian terrain. By deploying a swarm of more than 90 rovers equipped with various scientific instruments, this mission will significantly enhance our understanding of Mars, facilitating future human exploration and settlement.

The search for water in various forms is the common thread that binds the science goals of Mars exploration missions over the past few decades. For large scale water extraction (aimed at producing propellant and potable water in sizable quantities), a coordinated prospecting and characterisation campaign is required to arrive at maps of exploitable reserves.

Unfortunately, current architectures rely primarily on large, complex, and expensive rovers. While these platforms provide invaluable data, they are limited in their spatio-temporal coverage. Consequently, optimal Exploration Zones (EZs) for human exploration of Mars are yet to be defined.

Based on current priorities in Mars science and exploration, as well as the technical constraints of the Tumbleweed rover, a preliminary list of instruments was drafted. Exploring the synergies amongst these instruments, we arrived at the opportunity to use radiation-focused instrumentation to simultaneously achieve high-resolution mapping of hydrogen in the near-surface environment. Measuring the flux of epithermal neutron emissions is one of the best approaches towards estimating water equivalent hydrogen (WEH) abundance. Thermal and epithermal neutron measurements from instruments such as FREND, HEND and DAN have indicated the presence of WEH in the near-surface. This would represent the prime target for ISRU operations in the near future. However, the resolution of existing orbital maps of water ice is insufficient to direct and execute robotic/human operations on ground. 

This suite of radiation detection instruments will be consolidated in the future through the addition of a miniaturized Gamma Ray Spectrometer, providing the ability to perform elemental mapping along the rover traverse. Beyond neutron spectrometers, patch permittivity sensors may also be deployed on the Tumbleweed Rovers, enabling cross-confirmation of WEH mapping.

This instrumentation and our mission architecture enable high-resolution mapping of Martian environments, combining radiation scouting with WEH prospecting, thus identifying low-radiation and high-WEH regions ideal for crewed missions.

To aid further maturation and design of the mission, a conceptual study is proposed herein. Starting from a simulation of the individual rover’s trajectories on the surface of Mars, we shall geospatially compute the probable intersections with the already identified EZs on Mars. Based on these intersections we can infer thresholds for the controlled navigation of individual rovers (assessing intersections per trajectory buffer size) and classify candidate EZs according to known topography and available WEH mapping. This classification would enable more precise GEANT4 modelling of individual rovers and their instrumentation, resulting in probable neutron counts and dose/flux readings, leading to mission-specific requirements for our spacecrafts and their payloads.

How to cite: de Pinto Balsemão, M., Shanbhag, A., Kingsnorth, J., Bounova, G., Pikulić, L., Moisuc, C., Molhuijsen, D., and Rothenbuchner, J.: Mars Radiation Environment and Water-ice Prospecting through a Distributed Swarm of Tumbleweed Rovers , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19534, https://doi.org/10.5194/egusphere-egu25-19534, 2025.

EGU25-19713 | ECS | Posters on site | GI4.4

Understanding the influence of landscape heterogeneities on the signal of cosmic-ray neutron sensors by means of site-specific neutron transport simulation 

Jannis Weimar, Markus Köhli, Martin Schrön, Sascha Oswald, and Miroslav Zboril

Monitoring soil moisture is a challenging task due to its complex spatial patterns. In recent years, cosmic-ray neutron sensing has gained popularity for its ability to provide integral measurements over a few hectares horizontally and a few decimeters vertically, covering a representative volume for many research questions in various landscapes. However, interpreting signals using averaging methods becomes increasingly difficult as the heterogeneity of the observable increases.
As part of the SoMMet project, three field sites in Germany and Italy equipped with cosmic-ray neutron sensors are analyzed in detail using the Monte Carlo code URANOS. The virtual representation of these sites in the code allows for removing and adding structures. Thereby, all features of the landscape of the three different sites can be examined separately with respect to their impact on the local neutron field. These include general landscape heterogeneities, buildings, land use, and biomass. While this study focuses on three specific, although relatively common, site setups, it also offers general insights that can enhance the understanding of signal and footprint dynamics at other locations.

How to cite: Weimar, J., Köhli, M., Schrön, M., Oswald, S., and Zboril, M.: Understanding the influence of landscape heterogeneities on the signal of cosmic-ray neutron sensors by means of site-specific neutron transport simulation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19713, https://doi.org/10.5194/egusphere-egu25-19713, 2025.

EGU25-6148 | Posters on site | GI4.5

HALO airborne measurements; PERCUSION’s contribution to EarthCARE validation 

Silke Gross, Florian Ewald, Martin Wirth, André Ehrlich, Lutz Hirsch, Konstantin Krüger, Anna Luebke, Bernhard Mayer, Sophie Rosenburg, Lea Volkmer, Manfred Wendisch, Julia Windmiller, and Bjorn Stevens

In May 2024 the EarthCARE satellite mission EarthCARE was launched. For the first time, the satellite combines a high spectral resolution lidar and a cloud radar with doppler capability as key instruments on one single platform. In addition, it is equipped with a multi spectral imager and a broadband radiometer. This unique combination makes EarthCARE the most complex satellite mission to study aerosol, clouds, precipitation, and radiation. To fully use these new and advanced data for science applications, a careful validation of the measurements and data products is required. We have implemented an EarthCARE-like payload onboard the German research aircraft HALO (High Altitude and LOng range) to prepare and validate the EarthCARE data. This instrumentation was flown during PERCUSION (Persistent EarthCARE underflight studies of the ITCZ and organized convection) as a contribution to ORCESTRA (Organized Convection and EarthCARE Studies over the Tropical Atlantic).

ORCESTRA is a network of different campaigns conducted to better understand the organized tropical convection at the mesoscale, e.g. including the interaction of convective organization with tropical waves and air-sea interaction, and the impact of convective organization on the Earth’s climate and radiation budget. In addition, ORCESTRA helps to validate satellite remote sensing (especially EarthCARE). To achieve these objectives, ORCESTRA combines several sub-campaigns taking place on the Cape Verde Islands and Barbados in August and September 2024.

One of the campaigns within ORCESTRA is the PERCUSION campaign. PERCUSION aims to test factors hypothesized to influence the organization of deep maritime convection in the tropics and the influence of convective organization on its larger-scale environment. One focus of PERCUSION was to establish confidence in the EarthCARE measurements and products. For this purpose, we conducted one EarthCARE underpass within each research flight HALO measurements were performed during the EarthCARE commissioning phase in August 2024 out of Sal, Cape Verde, and out of Barbados in September 2024. In addition, we performed flights out of Oberpfaffenhofen, Germany in November 2024 for validation of conditions that could not be captured in the two first campaign parts. Altogether, 33 EarthCARE underpasses were carried out in different aerosol and cloud situations. Some of the flights were coordinated with in-situ measurements onboard other aircrafts (e.g. the French ATR42), with shipborne measurements onboard the German research vessel METEOR, or with ground-based radar and lidar measurements at Mindelo (Cape Verde), Barbados, and the ACTRIS stations Antikythera, Leipzig, Lindenberg and Munich. Four underpasses under NASA’s PACE mission were also performed.

In our presentation we will give an overview of ORCESTRA with the main focus on PERCUSION. We will present the HALO PERCUSION measurements and will show first comparisons of HALO lidar and radar and EarthCARE lidar and radar measurements.

How to cite: Gross, S., Ewald, F., Wirth, M., Ehrlich, A., Hirsch, L., Krüger, K., Luebke, A., Mayer, B., Rosenburg, S., Volkmer, L., Wendisch, M., Windmiller, J., and Stevens, B.: HALO airborne measurements; PERCUSION’s contribution to EarthCARE validation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6148, https://doi.org/10.5194/egusphere-egu25-6148, 2025.

EGU25-7050 | Orals | GI4.5

Spectroradiometric and Stray light characterization of the Pushbroom Imager for Cloud and Aerosol Research and Development (PICARD) Airborne Imager 

Alok Shrestha, Tom Ellis, Roseanne Domingues, Gary Hoffmann, Haiping Su, James Jacobson, Kerry Meyer, Julia Barsi, and Steven Platnick

The PICARD (Pushbroom Imager for Cloud and Aerosol Research and Development) instrument, developed by the NASA Ames Research Center in partnership with Brandywine Photonics, LLC, is an airborne imager consisting of dual Offner spectrometers and an all-reflective telescope with a 50° full field-of-view (FOV). The instrument operates over a wavelength range of 400 – 2400 nm in more than 200 bands. PICARD has already flown multiple engineering flights on NASA ER-2 high altitude aircraft, the most recent during 2023 Western Diversity Time Series (WDTS) spring campaign where near co-incident measurements with spaceborne sensors such as MODIS and VIIRS were obtained including those over railroad valley (RRV) calibration site.  In addition, PICARD has recently flown during the 2024 Plankton, Aerosol, Cloud, Ocean Ecosystem Postlaunch Airborne eXperiment (PACE-PAX) field campaign to gather data for the validation of the recently launched PACE mission. A recent analysis comparing PICARD measurements with RadCalNet dataset from RRV revealed excellent agreement for most of the bands except in the UV and blue region, where PICARD generally under reported. To better characterize these bands and improve this under reporting, detailed PICARD spectroradiometric characterization measurements were collected at Goddard Laser for Absolute Measurement of Radiance (GLAMR) laboratory at Goddard Space Flight Center (GSFC) in February 2024. The initial analysis of this characterization suggested that this under-report during flight is due to a stray light sensitivity inherent in the low signal-to-noise (SNR) bands of array spectroradiometers. Correcting for the GLAMR measured stray light reconciles the under report. In addition, poor SNR bands in SWIR atmospheric absorptions are recovered when corrected for stray light. In this presentation, we will share findings from our recent PICARD spectroradiometric characterization over GLAMR including updated results comparing PICARD flight radiances with RadCalNet at RRV.

How to cite: Shrestha, A., Ellis, T., Domingues, R., Hoffmann, G., Su, H., Jacobson, J., Meyer, K., Barsi, J., and Platnick, S.: Spectroradiometric and Stray light characterization of the Pushbroom Imager for Cloud and Aerosol Research and Development (PICARD) Airborne Imager, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7050, https://doi.org/10.5194/egusphere-egu25-7050, 2025.

EGU25-7774 | Posters on site | GI4.5

In-Situ Hyperspectral Absorption and Backscattering Sensors for Ocean Color and Biogeochemistry Research 

Kirby Simon, Wayne Slade, Christopher Strait, Alberto Tonizzo, Michael Twardowski, Thomas Leeuw, Chuck Pottsmith, Ravi Chandrasiri, and Ole Mikkelsen

Accurate measurements of in-water inherent optical properties (IOPs) such as absorption and backscattering, along with coincident in-situ and satellite-measured radiometry, are key to refining and calibrating algorithms used by hyperspectral satellite missions such as NASA PACE to derive ocean color data products. The accuracy of hyperspectral ocean color products, such as phytoplankton community composition, is therefore linked to the accuracy of in-situ IOP measurements. However, current instrumentation for in-situ absorption and backscattering measurements has been limited to either single- or multi-spectral wavelengths or to hyperspectral wavelengths that do not entirely meet the wavelength range and resolution requirements of PACE and other hyperspectral remote sensing missions. Advancements in instrumentation are therefore necessary to expand the range, resolution, and sensitivity of in-situ absorption and backscattering measurements to support these missions and the development and distribution of accurate ocean color data products. Additionally, advancements in hyperspectral absorption and backscattering sensors can offer new insights into studying particulate and dissolved materials in the ocean in support of biogeochemistry research.

We have recently developed and commercialized submersible hyperspectral absorption (Hyper-a) and backscattering (Hyper-bb) instruments to meet the needs of current (e.g., PACE) and future (e.g., GLIMR, SBG) hyperspectral remote sensing missions. The Hyper-bb is a single-angle backscatter sensor that utilizes a broadband LED source, scanning linear variable filter assembly, and sensitive photomultiplier tube detector. The Hyper-a is an absorption sensor that utilizes a xenon flash lamp, dual spectrometers (signal and reference), and a pump-through Lambertian integrating cavity that reduces measurement uncertainty due to scattering errors characteristic in a reflective tube design. Both sensors are designed to enable user calibration, reducing cost and downtime typically associated with sending the instrument back for factory calibration.

We will present details related to the development of these two hyperspectral instruments as well as their engineering specifications and recent test results from laboratory studies and field work.

How to cite: Simon, K., Slade, W., Strait, C., Tonizzo, A., Twardowski, M., Leeuw, T., Pottsmith, C., Chandrasiri, R., and Mikkelsen, O.: In-Situ Hyperspectral Absorption and Backscattering Sensors for Ocean Color and Biogeochemistry Research, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7774, https://doi.org/10.5194/egusphere-egu25-7774, 2025.

EGU25-7777 | Orals | GI4.5

Simultaneous aerosol and ocean retrievals from PACE multi-angle polarimeters: data products and validation 

Meng Gao, Kirk Knobelspiesse, Bryan Franz, Peng-wang Zhai, Kamal Aryal, Andrew Sayer, Amir Ibrahim, and Jeremy Werdell

The NASA Plankton, Aerosol, Cloud, ocean Ecosystem (PACE) mission, successfully launched on February 8, 2024, with aims to advance our understanding of global ocean ecology, biogeochemistry, atmospheric aerosols, and clouds. PACE features cutting-edge instruments, including the Ocean Color Instrument (OCI), a hyperspectral scanning radiometer, and two Multi-Angle Polarimeters (MAPs): the UMBC Hyper-Angular Rainbow Polarimeter (HARP2) and the SRON Spectro-Polarimeter for Planetary EXploration one (SPEXone). These instruments offer valuable data for simultaneous retrievals of aerosol, cloud, and surface properties.

This talk will focus on simultaneous aerosol and ocean retrievals derived from PACE MAP measurements, emphasizing data products, uncertainties, and validation. The retrieved products encompass aerosol properties such as complex refractive index, effective radius and variance, layer height, optical depth, and single-scattering albedo, as well as oceanic and surface properties. To streamline operational processing, we have incorporated deep neural network-based radiative transfer models into the PACE polarimetric retrieval algorithms via the FastMAPOL framework. Preliminary validation against in-situ measurements will be presented, along with potential applications of MAP data, including the study of ocean color bidirectional reflectance signals and multi-angle cloud masking.

How to cite: Gao, M., Knobelspiesse, K., Franz, B., Zhai, P., Aryal, K., Sayer, A., Ibrahim, A., and Werdell, J.: Simultaneous aerosol and ocean retrievals from PACE multi-angle polarimeters: data products and validation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7777, https://doi.org/10.5194/egusphere-egu25-7777, 2025.

EGU25-7979 | Posters on site | GI4.5

Heat-island-effect of ship-based bulk measurements for evaporation duct estimation 

Xiaofeng Zhao, Yuxing Wang, Pinglv Yang, Yibin Chen, and chunshan Wei

Because the evaporation duct profile is difficult to measure, different empirical surface layer models have been developed to compute the average refractivity profile near the ocean surface using four bulk measurements: pressure, temperature, humidity, wind speed at a single height (e.g., the ship’s bridge), and sea surface temperature (SST). Although these parameters can be conveniently measured using standard equipment, the measurement accuracy is usually influenced by inherent factors, such as the movement of the ship or the heat island effect. To analyze the heat island effect of ship-based bulk measurements for evaporation duct estimation, an open cruise observation over the Tropical Eastern Indian Ocean from 23 Aug 2024 to 14 Oct 2024 is used. The ship weather station measurements and the corresponding evaporation duct profiles, computed by the NPS evaporation duct model, are compared with 48 low-altitude rocketsonde profiles, which sample a high vertical resolution of air temperature, air humidity, air pressure, and wind parameters. The sensors for air temperature, humidity, pressure, and wind vector are deployed at 13.4 m above the mean sea level, and the SST is measured by an infrared thermometer. The results show that the mean air temperature and relative humidity of the ship measurements are 1.03 K and 4.07% higher than the rocketsonde measurements at the same altitude (i.e., 13.4 m), and the evaporation duct height and strength computed from the ship-based measurements are 1.98 m and 10.07 M-units lower than those from the rocketsonde measurements.

How to cite: Zhao, X., Wang, Y., Yang, P., Chen, Y., and Wei, C.: Heat-island-effect of ship-based bulk measurements for evaporation duct estimation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7979, https://doi.org/10.5194/egusphere-egu25-7979, 2025.

EGU25-8293 | Posters on site | GI4.5

Radiometric Calibration using Artificial Intelligence: Constituting Uniform Observing Systems for Infrared Satellites 

Boyang Chen, Aiqun Wu, Wen Hui, Peng Rao, Xuang Feng, Fansheng Chen, Changpei Han, Qichao Ying, Yapeng Wu, Miao Liu, Damian Moss, and Zhenxing Qian
Radiometric Calibration (RC) is a critical process in aerospace infrared remote sensing that establishes the relationship between the radiation energy of observed objects and the Digital Number (DN) output from sensors, which is fundamental for ensuring high-precision applications of infrared remote sensing data. At present, Source-Based RC (SBRC) is the predominant method, relying on a variety of Radiometric Sources (RS) including in-orbit blackbodies, or natural targets such as lakes, oceans. This approach, while effective, imposes constraints on remote sensing systems such as space & weight allocation for RS and additional observation time for RC. Moreover, the reliance on physical calibration sources can introduce uncertainties due to factors such as imperfect emissivity of in-orbit blackbodies, lack of data consistency due to varied RS types, and variations in environmental conditions. In this paper, we propose a novel RC method named Artificial Intelligence Radiometric Calibration (AIRC), which directly generates RC coefficients for the in-orbit remote sensing satellites using the physical and environmental parameters of the sensor. We first theoretically prove that RC coefficients can be derived as functions of the sensor states. Next, we propose our Neural Networks for infrared Radiometric Calibration (RCNN), to learn this relationship based on historical high-accuracy calibration data, enabling a shift from Reference Traceability (RT) to States Traceability (ST). Then, to verify the feasibility of the proposed scheme, we train and test an Multi-layered Perceptron (MLP) as a simple implementation of RCNN based on our long-term well-curated RC data from our FengYun-4A Avanced Geosynchronous Radiation Imager (FY-4A AGRI), and the experiments show that the proposed method achieves high-accuracy RC comparable with the official RC method applied on FY-4A AGRI that uses an in-orbit blackbody. Our study showcases how to conduct RC using the “reason (the states of sensor) - results (calibration coefficient)” logic, as supplement to the existing “result (observation to RS) - reason (calibration coefficient)” logic, which promotes constituting a uniform observing system for cross-platform infrared satellites.

How to cite: Chen, B., Wu, A., Hui, W., Rao, P., Feng, X., Chen, F., Han, C., Ying, Q., Wu, Y., Liu, M., Moss, D., and Qian, Z.: Radiometric Calibration using Artificial Intelligence: Constituting Uniform Observing Systems for Infrared Satellites, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8293, https://doi.org/10.5194/egusphere-egu25-8293, 2025.

EGU25-8313 | Posters on site | GI4.5

Advanced cloud products from NASA’s PACE mission 

Bastiaan van Diedenhoven, Chamara Rajapakshe, Andrzej Wasilewski, Andrew Sayer, Brian Cairns, Otto Hasekamp, Kirk Knobelspiesse, Mikhail Alexandrov, Daniel Miller, Kenneth Sinclair, Brent McBride, and Vanderlei Martins

The sensitivities of cloud properties to changes in the climate and to anthropogenic aerosol emissions are crucial for understanding Earth’s climate but remain highly uncertain. Global cloud observations from satellites are needed to advance our knowledge on processes related to the formation and evolution of clouds and precipitation. While long term satellite data records of cloud microphysical properties exist, largely obtained by multi-spectral imagers, they are known to be substantially biased or failing in particular situations, such as in regions of broken and/or mixed-phase clouds. The cloud products provided by NASA’s Plankton, Aerosol, Cloud, ocean Ecosystem (PACE) mission, which was launched on 8 February 2024, have several advantages over past missions. PACE caries the Ocean Color Instrument (OCI), which is a multi-spectral imager, the Hyper-angular Rainbow Polarimeter (HARP-2) and the Spectropolarimeter for Planetary Exploration (SPEXone). Advanced, pixel-level cloud microphysical products are produced from the polarimeters, including cloud top phase and full droplet size distributions, while collocated retrievals are provided by OCI using more traditional methods. Instrument-synergy products include liquid water path and droplet number concentrations. We present first global advanced cloud products from PACE. We present validation using airborne campaigns that indicates that the polarimetry products are much less affected by the presence of broken and mixed-phase clouds than OCI observations, consistent with previous studies using simulations and observations. These observations provide new insights on the microphysical properties of global clouds, including their drop size distribution width and bi-modality which may be linked to precipitation formation. Furthermore, we show that the polarimeter retrievals along with OCI’s unique combination of three commonly-used shortwave infrared wavelength bands allows to assess some of the biases in traditional bi-spectral retrievals in unprecedented detail and on a global scale. We show that the biases in bi-spectral results depend on cloud structure and on the wavelength used for the droplet size retrievals. The PACE data provides crucial information to reduce biases in traditional bi-spectral cloud retrievals by essentially all multi-spectral imagers in the program of record that result from, e.g., sub-pixel cloudiness, mixed-phase cases and 3D radiative transfer effects. We make recommendations on how biases in bi-spectral results may be mitigated.

How to cite: van Diedenhoven, B., Rajapakshe, C., Wasilewski, A., Sayer, A., Cairns, B., Hasekamp, O., Knobelspiesse, K., Alexandrov, M., Miller, D., Sinclair, K., McBride, B., and Martins, V.: Advanced cloud products from NASA’s PACE mission, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8313, https://doi.org/10.5194/egusphere-egu25-8313, 2025.

EGU25-9811 | Orals | GI4.5

ACROSS Mediterranean activities for EarthCARE validation and exploitation 

Eleni Marinou and the ACROSS team

The ESA-JAXA EarthCARE satellite mission, launched in May 2024, delivers vertical profiles of aerosols, clouds, and precipitation properties together with radiative fluxes, utilizing an instrumental suite of a high spectral resolution lidar (ATLID), a Doppler cloud radar (CPR), a multi-spectral imager (MSI), and a broadband radiometer (BBR). The simultaneous measurements will be utilized to improve our understanding of aerosol-cloud interactions (ACI) and their radiative effects and to assess the representation of clouds, precipitation, aerosols, radiative fluxes, and heating rates in weather and climate models [1]. Due to the multi-sensor complexity/diversity and the innovation of its standalone and synergistic products, the EarthCARE mission has several validation challenges and strong sub-orbital synergies are needed to address Cal/Val and science objectives.

The Mediterranean basin provides a complex aerosol-cloud environment for the exploitation EarthCARE's capabilities. For the validation of the EarthCARE products in the Mediterranean, the ACROSS validation activity will be implemented, which would increase synergies towards achieving the following objectives: (i) validate EarthCARE aerosol and cloud products using state-of-the-art ground-based and airborne facilities, (ii) implement science studies targeting radiative closures, ACI, and data assimilation experiments, (iii) and provide information for harmonizing and bridging past and future missions, to deliver Climate Data Records on aerosols and clouds.

The rationale for ACROSS is based on lessons learned from the JATAC campaign in the Atlantic [2]. Following the JATAC example, we target to implement 3 Intensive Observational Periods, including large-scale field experiments in the Mediterranean. The suborbital component follows the ASKOS [3] example. It includes (i) ACTRΙS Aerosol and Cloud remote sensing facilities and high-precision radiation measurements (Potenza site in Italy, Limassol Cyprus, as well as Pyrgos, Thessaloniki, and PANGEA sites in Greece), (ii) radiation measurements for closure studies, (iii) UAV and aircraft in-situ flights collocated with the remote sensing measurements. ACROSS activities will be clustered with the ARCHIMEDES experimental activities in the Mediterranean, foreseen between late 2026 and late 2027. ACROSS seeks synergies with airborne activities. To this end, the first synergistic measurements were collected during the PERCUSION campaign in November 2024, during which HALO underpass two EarthCARE tracks close to the Thessaloniki and PANGEA sites. More airborne activities are envisioned in the Mediterranean area for Spring/September 2025/2026.

ACROSS is a collaborative effort between NOA, DLR, the University of Nova Gorica, CyI, INOE, FMI, CNR-IMAA, PMOD, ERATOSTHENES CoE, CUT, and TROPOS. ACROSS is supported by ACTRIS RI and the dataset collected will support assimilation experiments and science activities in the framework of the PANGEA4CalVal, ATMO-ACCESS, and CERTAINTY EC projects and collaborations within.

References:

[1] Wehr T. et al., https://doi.org/10.5194/amt-16-3581-2023, 2023.

[2] Fehr, T., et al., https://doi.org/10.5194/egusphere-egu23-7249, 2023. 

[3] Marinou, E. Et al., https://doi.org/10.3390/environsciproc2023026200, 2023.

Acknowledgments: This research was financially supported by the PANGEA4CalVal project (Grant Agreement 101079201) funded by the European Union, and the CERTAINTY project (Grant Agreement 101137680) funded by the Horizon Europe program. Part of the wok was financed through the Core Program within the Romanian National Research Development and Innovation Plan 2022-2027, carried out with the support of MCID, project no. PN 23 05.

How to cite: Marinou, E. and the ACROSS team: ACROSS Mediterranean activities for EarthCARE validation and exploitation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9811, https://doi.org/10.5194/egusphere-egu25-9811, 2025.

EGU25-11760 | ECS | Orals | GI4.5

Aerosol Validation in NASA's PACE mission: Deployment of the SPEX Airborne Polarimeter in the PACE-PAX Field campaign 

Brecht Simon, Jasper Mens, Martijn Smit, Guangliang Fu, Jeroen Rietjens, Martin Grim, Tim Vonsée, Jelle Talsma, Rob Wolfs, Otto Hasekamp, and Bastiaan van Diedenhoven

The Plankton, Aerosol, Cloud, Ocean Ecosystem Postlaunch Airborne eXperiment (PACE-PAX) is a multi-platform, multi-instrument field campaign designed to validate NASA’s PACE mission. Two research aircraft participated in this month-long campaign: the CIRPAS Twin Otter, conducting in situ observations of aerosols and clouds, and NASA’s high-altitude research aircraft ER-2, equipped with remote sensing instruments. Among these instruments is SPEX airborne, an airborne proxy for the Dutch SPEXone instrument onboard PACE. SPEX airborne, like SPEXone, is a multi-angle spectropolarimeter for wavelengths between 400 and 780 nm, designed to characterize aerosols in the Earth’s atmosphere. It has nine viewing angles (nadir, ±14°, ±28°, ±42°, and ±56°) and an across-track swath of about 2.1 km at nadir at nominal ER-2 flight altitudes. SPEX airborne radiance and polarization data are formatted identically to SPEXone data, enabling the use of the same RemoTAP algorithm to retrieve aerosol properties such as aerosol optical depth, size distributions, refractive index, layer height, and composition. During multiple flights, totaling over 80 flight hours, the ER-2 frequently flew under PACE and ESA’s EarthCARE satellite, as well as over the Twin Otter, calibration sites, and aerosol ground stations, facilitating extensive data comparisons. In this presentation, we present preliminary validation of publicly released SPEX airborne level-1 data and collocate these with SPEXone observations. Additionally, we present validation of SPEX airborne aerosol retrievals against AERONET stations and other instruments deployed during PACE-PAX. The RemoTAP aerosol retrievals from SPEX airborne data emphasize the key role of PACE-PAX in confirming aerosol properties derived from SPEXone.

How to cite: Simon, B., Mens, J., Smit, M., Fu, G., Rietjens, J., Grim, M., Vonsée, T., Talsma, J., Wolfs, R., Hasekamp, O., and van Diedenhoven, B.: Aerosol Validation in NASA's PACE mission: Deployment of the SPEX Airborne Polarimeter in the PACE-PAX Field campaign, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11760, https://doi.org/10.5194/egusphere-egu25-11760, 2025.

EGU25-12925 | ECS | Posters on site | GI4.5

From PACE to PLACE: Results from the First Months of Land Data Products 

Skye Caplan, Antonio Mannino, Morgaine McKibben, Fred Huemmrich, Kirk Knobelspiesse, Jeremy Werdell, Meng Gao, Otto Hasekamp, and Guangliang Fu

Although “land” is not included the acronym for NASA’s Plankton, Aerosol, Cloud, ocean Ecosystem (PACE) satellite, the mission is actively supporting terrestrial science. Two new global, daily product suites were recently released using land data from PACE’s Ocean Color Instrument (OCI). The first, termed SFREFL, is a hyperspectral collection of surface reflectances from the ultraviolet into the shortwave infrared. SFREFL currently employs L2gen for atmospheric correction, ensuring continuity with heritage missions processed by the Ocean Biology Processing Group. ISOFIT is also being considered for use as a standard surface reflectance algorithm. Both algorithms make PACE terrestrial data directly applicable to future hyperspectral missions like SBG, and ease collaboration with current missions producing similar products. The second suite, LANDVI, includes 10 vegetation indices: 6 multispectral (NDVI, EVI, NDWI, NDII, CCI, and NDSI) and 4 which are hyperspectral-enabled, or narrowband (PRI, Car, CIRE, and mARI). Narrowband indices leverage OCI’s unique capabilities to provide previously uncharacterized insights into the status of terrestrial ecosystems across the globe. Having been in production for several months, preliminary results from both SFREFL and LANDVI will be presented here. The integration of these terrestrial products as outputs from PACE positions the mission as pivotal for global environmental monitoring and establishes it as an important part of the terrestrial hyperspectral data record.

How to cite: Caplan, S., Mannino, A., McKibben, M., Huemmrich, F., Knobelspiesse, K., Werdell, J., Gao, M., Hasekamp, O., and Fu, G.: From PACE to PLACE: Results from the First Months of Land Data Products, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12925, https://doi.org/10.5194/egusphere-egu25-12925, 2025.

EGU25-12978 | Orals | GI4.5

NASA’s PACE Mission Status Updates: Advancing Science and Data Products 

Amir Ibrahim, Jeremy Werdell, Ivona Cetinic, Bryan Franz, Brian Cairns, Susanne Craig, Otto Hasekamp, Antonio Mannino, Vanderlei Martin, Gerhard Meister, and Andrew Sayer

Following its launch from Kennedy Space Center in February 2024, NASA’s Plankton, Aerosol, Cloud, ocean Ecosystem (PACE) mission has been revolutionizing our understanding of Earth’s systems. The observatory hosts three cutting-edge instruments: the Ocean Color Instrument (OCI), a hyperspectral radiometer, and two multi-angular polarimeters, SpexOne and HARP2. Together, these instruments are collecting unprecedented data on our living oceans, atmospheric aerosols and clouds, and land.

PACE extends NASA’s legacy of over 20 years of global satellite observation while initiating an advanced suite of climate-relevant data records. For the first time, daily global measurements are enabling improved predictions of fisheries dynamics, the emergence of harmful algal blooms, and other critical factors impacting commercial and recreational industries. Furthermore, PACE provides key insights into cloud properties and aerosols—tiny airborne particles that influence air quality and regulate Earth's energy balance by absorbing and reflecting sunlight.

Since its launch, the PACE science team, in collaboration with the broader scientific community, has focused on implementing, testing, and validating mission data products. Performance assessments through the PACE Validation Science Team (PVST) and field campaigns, such as the Post-launch Airborne eXperiment (PACE-PAX), have been pivotal in refining data quality and enhancing the mission’s scientific outcomes.

This presentation provides an overview of the current status of PACE science products, highlighting key achievements, ongoing validation efforts, and future goals aimed at maximizing the mission’s contributions to Earth science.

How to cite: Ibrahim, A., Werdell, J., Cetinic, I., Franz, B., Cairns, B., Craig, S., Hasekamp, O., Mannino, A., Martin, V., Meister, G., and Sayer, A.: NASA’s PACE Mission Status Updates: Advancing Science and Data Products, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12978, https://doi.org/10.5194/egusphere-egu25-12978, 2025.

EGU25-13069 | Posters on site | GI4.5

PACE Mission validation with the PACE-PAX field campaign 

Ivona Cetinic, Kirk Knobelspiesse, Brian Cairns, and Jeremy Werdell

NASA's Plankton, Aerosol, Clouds, and Ocean Ecosystems (PACE) Mission, launched a year ago, provides data on ocean color, aerosols, clouds, and land surfaces through its three advanced sensors. Some of these data products rely on established "heritage" algorithms, ensuring continuity with previous and ongoing missions, while others are novel, leveraging recent algorithmic advancements and PACE's unique measurement capabilities. To validate PACE's data products, the PACE Postlaunch Airborne eXperiment (PACE-PAX) was conducted in September 2024 in California. This campaign featured coordinated operations involving multiple aircraft, ocean vessels, and surface-based instruments, particularly timed with PACE satellite overpasses. Additionally, PACE-PAX supported similar activities for ESA's EarthCARE (Cloud, Aerosol, and Radiation Explorer) Mission. This presentation highlights the campaign's achievements, discusses the current status of the data, and outlines future plans for utilizing this valuable dataset.

How to cite: Cetinic, I., Knobelspiesse, K., Cairns, B., and Werdell, J.: PACE Mission validation with the PACE-PAX field campaign, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13069, https://doi.org/10.5194/egusphere-egu25-13069, 2025.

EGU25-13336 | ECS | Posters on site | GI4.5

PACE Applications Program: Putting PACE remote sensing data to work for societal benefit across the Earth System  

S. Morgaine McKibben and Skye Caplan

Launched in February 2024 and serving data to the public as of April 2024, the NASA Plankton, Aerosol, Cloud, ocean Ecosystem (PACE) satellite provides a novel set of hyperspectral and polarimetric Earth observation (EO) capabilities across aquatic, terrestrial, and atmospheric domains-- an interdisciplinary span not matched by other EO missions. With these observations, PACE data can support multiple applications areas such as water resource management, public health and air quality, climate science, terrestrial and agricultural, post-disaster monitoring, and more. The PACE Applications Program has the primary goal of fostering and accelerating the translation of PACE’s advanced data into actionable applications that benefit society. To achieve this, we support bridging of researchers and applied end users through programming such as the PACE Community of Practice, Early Adopters Program, and information-sharing and co-production activities such as workshops and focus sessions. In this presentation we describe the interdisciplinary applications capabilities of PACE and opportunities for you to engage with our program.

How to cite: McKibben, S. M. and Caplan, S.: PACE Applications Program: Putting PACE remote sensing data to work for societal benefit across the Earth System , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13336, https://doi.org/10.5194/egusphere-egu25-13336, 2025.

EGU25-14131 | Orals | GI4.5

First comparison between EarthCARE’s CPR and airborne W-band cloud radar observations during ECALOT campaign 

Paloma Borque, Cuong Nguyen, Zhipeng Qu, Pavlos Kollias, Bernat Puigdomenech, Keyvan Ranjbar, Kenny Bala, Natalia Bliankinshtein, Leonid Nichman, Sudesh Boodoo, and Norman Donaldson

Improving future climate predictions requires enhancing the current meteorological numerical models for which a better understanding of the roles that clouds and aerosols (and their interactions) play in Earth’s weather and climate is crucial.  Along these lines, the European Space Agency (ESA) and the Japan Aerospace Exploration Agency (JAXA) successfully launched the Earth Cloud, Aerosol, and Radiation Explorer (EarthCARE) satellite in May 2024. This satellite mission aims to advance the studies of global aerosol and cloud properties via novel active and passive spaceborne observations.  EarthCARE carries four instruments: the ATmospheric LIDar (ATLID), the Cloud Profiling Radar (CPR), the Multi-Spectral Imager (MSI), and the Broadband Radiometer (BBR).  Of particular interest to this work are the CPR observations providing significant observations of clouds’ vertical structure, including the first ever in-cloud Doppler Velocity profiles from space.

As part of ESA’s global calibration/validation initiative, the EarthCARE Commissioning Calibration/Validation Campaign in Ottawa (ECALOT) took place in Canada from October 2024 to January 2025.  ECALOT collected essential airborne and surface observations to calibrate and validate key EarthCARE products. These include CPR and ATLID Level 1 and Level 2 products, composite and synergy products, as well as EarthCARE’s scene construction algorithm and radiation products.  ECALOT successfully observed fall and winter weather conditions with dedicated flights targeted to sample relevant weather underflying the EarthCARE path.  The National Research Council Canada’s (NRC) Convair-580 aircraft, equipped with W- and X- band radars (NAWX), 355nm Lidars, and a full array of state-of-the-art in-situ cloud microphysics and aerosol probes, provided critical independent observations to support EarthCARE validation efforts.  These observations were complemented by surface-based sites deployed by Environment and Climate Change Canada and McGill University near Ottawa airport and two Climate Sentinels network stations operated by McGill University and Université du Québec à Montréal in the Montreal region.

In this presentation, we will provide an initial evaluation of EarthCARE’s CPR performance during the ECALOT campaign.  A comprehensive analysis of the cloud vertical structure as seen by the CPR and NAWX observations and an intercomparison of vertical cross sections of reflectivity and Doppler velocity will be presented.  In addition, an assessment of the behavior of CPR under stratiform and convective conditions will be provided.

How to cite: Borque, P., Nguyen, C., Qu, Z., Kollias, P., Puigdomenech, B., Ranjbar, K., Bala, K., Bliankinshtein, N., Nichman, L., Boodoo, S., and Donaldson, N.: First comparison between EarthCARE’s CPR and airborne W-band cloud radar observations during ECALOT campaign, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14131, https://doi.org/10.5194/egusphere-egu25-14131, 2025.

EGU25-14414 | Posters on site | GI4.5

PACE Observatory validation plan, data sources, and results  

Inia M Soto Ramos, James Allen, Ivona Cetinić, Amir Ibrahim, Christopher W. Proctor, Kirk D. Knobelspiesse, and Jeremy Werdell

The success of Earth Science space-borne missions relies on the availability of optical field measurements, as well as a solid validation plan to assess and verify the in-orbit quality of the data products. Since the late 1990s, NASA’s SeaBASS has served the ocean color community as the primary repository for in situ radiometric and pigment observations, facilitating robust product validation across multiple missions. The PACE science data validation program is responsible for making sure data products meet mission-specified requirements and for assessing uncertainties across various water types, cloud conditions, and aerosol distributions. In addition to SeaBASS, the PACE validation plan includes 24 PACE Validation Science Teams and a targeted field campaign called PACE-PAX. Nonetheless, an ongoing challenge remains the limited number of matchups between in situ and satellite measurements due to cloud cover, data quality issues, and other constraints. Here, we discuss the limitations and challenges of ocean color validation and present the current PACE validation plan, data sources, and early validation results. 

How to cite: Soto Ramos, I. M., Allen, J., Cetinić, I., Ibrahim, A., Proctor, C. W., Knobelspiesse, K. D., and Werdell, J.: PACE Observatory validation plan, data sources, and results , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14414, https://doi.org/10.5194/egusphere-egu25-14414, 2025.

EGU25-14437 | ECS | Posters on site | GI4.5

The First Year of the Hyper-Angular Rainbow Polarimeter (HARP2) on the NASA PACE mission: Performance, Science, and Synergy 

Brent McBride, J. Vanderlei Martins, Xiaoguang Xu, Anin Puthukkudy, Roberto Fernandez-Borda, Noah Sienkiewicz, Rachel Smith, Meng Gao, Bastiaan van Diedenhoven, Snorre Stamnes, Kirk Knobelspiesse, Andrew Sayer, Chamara Rajapakshe, Bryan Franz, Frederick Patt, Carissa Arillo, Brian Cairns, Jeremy Werdell, and Lorraine Remer

Over the past year, the Hyper-Angular Rainbow Polarimeter (HARP2) multi-angle imaging polarimeter instrument on the NASA Plankton Aerosol Cloud ocean Ecosystem (PACE) mission observed the entire Earth every two days. HARP2 measures total and polarized radiances over four spectral channels (440/550/670/870 nm), at up to 90 distinct viewing directions, and over a 114° field-of-view (1550 km cross-track swath). This large volume of daily information requires new approaches to on-orbit operations, data processing, calibration, and science. In this work, we celebrate and recap the first year of HARP2 on PACE – from pre-launch to on-orbit calibration (solar/lunar/vicarious), exciting new and synergistic science products for cloud, aerosol, and ocean properties, and co-located intercomparisons with OCI, SPEXone, and AirHARP2 underflights during the recent NASA PACE-PAX field campaign. We close with a look ahead to HARP2 as a pathfinder for upcoming polarimetry missions.

How to cite: McBride, B., Martins, J. V., Xu, X., Puthukkudy, A., Fernandez-Borda, R., Sienkiewicz, N., Smith, R., Gao, M., van Diedenhoven, B., Stamnes, S., Knobelspiesse, K., Sayer, A., Rajapakshe, C., Franz, B., Patt, F., Arillo, C., Cairns, B., Werdell, J., and Remer, L.: The First Year of the Hyper-Angular Rainbow Polarimeter (HARP2) on the NASA PACE mission: Performance, Science, and Synergy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14437, https://doi.org/10.5194/egusphere-egu25-14437, 2025.

EGU25-15557 | Posters on site | GI4.5

Validation of Aerosol Products from Polarimetric Sensors – Application to PARASOL and 3MI 

Bertrand Fougnie, Soheila Jafariserajehlou, and David Huerta Valcarce

With the launch of EPS-SG in 2025, a new era for a long-term operational Near-Real-Time provision of aerosol product is starting. If most of the potential for such a new remote sensing polarimetry has been demonstrated since 1996 with the 3 POLDER and PARASOL missions, the recent advance in term of retrieval but also analysis and exploitation of the data reveal more and more the potential. Indeed, polarimeters allow the observation of aerosols with a significantly improved information content which will feed the retrieval. On top of the aerosol optical thickness classically retrieved, an additional set of parameters characterizing the aerosol properties can now be derived. This specificity of polarimeters requires a more demanding effort in term of validation. We will overview the different aspects to be considered for the validation, describe the methodology for most of the parameters, and focus on some examples.   

How to cite: Fougnie, B., Jafariserajehlou, S., and Huerta Valcarce, D.: Validation of Aerosol Products from Polarimetric Sensors – Application to PARASOL and 3MI, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15557, https://doi.org/10.5194/egusphere-egu25-15557, 2025.

EGU25-20586 | ECS | Orals | GI4.5

Liquid Water Cloud Retrievals from HARP2 and AirHARP2 Measurements from the PACE-PAX Validation Campaign 

Rachel Smith, Xiaoguang Xu, Brent McBride, and Vanderlei Martins

The Hyper Angular Rainbow Polarimeter 2 (HARP2), developed at UMBC, is a state-of-the-art wide field-of-view polarimeter capable of measuring total and polarized radiances with fine angular resolution (≥2 degrees) and high polarization accuracy in four spectral channels (440, 550, 670, 870 nm). HARP2 was successfully launched in February 2024 aboard NASA’s Plankton Aerosol Cloud and ocean Ecosystem (PACE) satellite and has since been collecting critical science data on Earth’s atmospheric, oceanic, and surface properties. In September 2024, UMBC’s AirHARP2, an advanced airborne polarimeter closely resembling the orbital HARP2, participated in the PACE Postlaunch Airborne eXperiment (PAX). This campaign provides a unique opportunity to validate radiometric and polarimetric measurements and derived science products from the PACE satellite by conducting direct cross-platform comparisons using co-located scenes. This study focuses on the retrieval comparisons of liquid water cloud microphysical properties from HARP2 and AirHARP2 during PACE-PAX using a novel look-up-table retrieval algorithm that leverages the geometric features of the polarized cloudbow to infer the cloud droplet size distribution. The retrievals will be performed using a novel look-up-table retrieval algorithm that uses the geometric parameters of the polarized cloudbow to retrieve the cloud droplet size distribution. With AirHARP2’s Level-1C grid resolution (~120 m) approximately 42 times finer than HARP2’s (~5 km), we will also examine the impact of spatial resolution on retrieval performance. The results will be further validated by cross-comparisons with official cloud products from the Ocean Color Instrument, the primary instrument aboard PACE.

How to cite: Smith, R., Xu, X., McBride, B., and Martins, V.: Liquid Water Cloud Retrievals from HARP2 and AirHARP2 Measurements from the PACE-PAX Validation Campaign, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20586, https://doi.org/10.5194/egusphere-egu25-20586, 2025.

EGU25-20694 | Posters on site | GI4.5

System Vicarious Calibration of the PACE Ocean Color Instrument 

Robert Frouin, Jing Tan, Andrew Barnard, Alexander Bailess, Emmanuel Boss, Nils Haëntjens, Andrew Banks, Paul Chamberlain, and Matthew Mazloff

System vicarious calibration (SVC) of satellite ocean-color sensors involves comparing retrievals of water-leaving radiance (Lw) with in-situ measurements at the time of overpass and adjusting the calibration coefficients to ensure agreement between retrieved and measured quantities. This approach is designed to reduce uncertainties associated with purely radiometric calibration techniques, which lack the accuracy required for science applications, and to minimize biases introduced by atmospheric correction. For the recently launched PACE Ocean Color Instrument (OCI), the methodology utilizes hyperspectral Lw measurements from HyperNav radiometer systems deployed at various locations (Crete, Moorea, Puerto Rico, Hawaii) and from the Marine Optical Buoy (MOBY) near Lanai. Match-ups are rigorously selected based on criteria for atmospheric, surface, water, and geometry conditions. Top-of-atmosphere (TOA) radiance derived from onboard calibration techniques is compared to TOA radiance calculated from in-situ Lw measurements, resulting in calibration adjustment gains. The application of these adjusted gains to OCI imagery in diverse oceanic regions demonstrates more realistic values for water reflectance, enhancing the accuracy of retrieved ocean color data for scientific analyses.

How to cite: Frouin, R., Tan, J., Barnard, A., Bailess, A., Boss, E., Haëntjens, N., Banks, A., Chamberlain, P., and Mazloff, M.: System Vicarious Calibration of the PACE Ocean Color Instrument, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20694, https://doi.org/10.5194/egusphere-egu25-20694, 2025.

Long-term, global ocean-color observations are needed for biogeochemistry and climate applications and require integration across multiple satellite sensors. This study proposes a methodology for cross-calibrating polar-orbiting ocean-color sensors using a geostationary reference sensor. The geostationary sensor serves as an intermediary, offering numerous coincidences in time and geometry with polar-orbiting sensors, particularly over oceanic regions where radiance levels are typical for ocean-color remote sensing. The methodology is applied to cross-calibrate current ocean-color sensors, including the recently launched OCI, using AHI, a sensor expected to remain stable over short cross-calibration intervals. Accuracy is evaluated based on radiometric noise, acquisition time differences, solar and viewing geometry variations, and spectral band mismatch uncertainties. Cross-calibration coefficients derived from suitable imagery provide a foundation for consistent, normalized calibration of polar-orbiting sensors, enabling the generation of reliable long-term ocean-color products from multiple satellites.

How to cite: Tan, J. and Frouin, R.: Cross-Calibration of Polar-Orbiting Satellite Ocean-Color Sensors Using a Geostationary Reference Sensor, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20712, https://doi.org/10.5194/egusphere-egu25-20712, 2025.

EGU25-629 | ECS | PICO | GM2.3

Leveraging Machine Learning for accurate and interpretable suspended sediment concentration predictions 

Houda Lamane, Latifa Mouhir, Rachid Moussadek, Bouamar Baghdad, and Ali El Bilali

Suspended sediment concentration (SSC) significantly impacts water quality, aquatic ecosystems, and reservoir capacity, making accurate prediction vital for effective watershed management. Traditional empirical and physically based models often struggle to handle the complexities and non-linear dynamics of sediment transport. Machine learning (ML) techniques, with their ability to model non-linear relationships and process large datasets, offer a promising alternative. This study explores the application of ML models, including extra trees (ET), random forest (RF), categorical boosting (CatBoost), and extreme gradient boosting (XGBoost) and their combination with genetic programming (GP), to predict SSC. Key environmental variables such as precipitation, streamflow, and seasonality are used as inputs, and the models are trained and validated using historical hydrological data. The SHapley Additive exPlanations (SHAP) framework is employed to interpret the models, offering insights into the influence of each input variable on SSC predictions. Results demonstrate that ML models outperform traditional approaches in accuracy and robustness, particularly in capturing peak sediment events. The findings underline the potential of ML in improving SSC prediction and guiding sustainable watershed management practices.

Keywords: Suspended Sediment Concentration (SSC), Machine Learning (ML), SHAP Values, Hydrological Modeling, Sediment Transport, Watershed Management.

How to cite: Lamane, H., Mouhir, L., Moussadek, R., Baghdad, B., and El Bilali, A.: Leveraging Machine Learning for accurate and interpretable suspended sediment concentration predictions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-629, https://doi.org/10.5194/egusphere-egu25-629, 2025.

EGU25-5869 | ECS | PICO | GM2.3

Network-scale modelling of bedload transport in Alpine rivers using D-CASCADE model 

Felix Pitscheider, Anne-Laure Argentin, Diane Doolaeghe, Mattia Gianini, Leona Repnik, Simone Bizzi, Stuart N. Lane, and Francesco Comiti

Quantifying sediment transport dynamics in Alpine rivers is essential for predicting their geomorphological evolution, for managing flood risks and fluvial ecosystems, as well as for sustainable management of hydropower schemes. However, actual data on sediment transport, particularly for the bedload fraction, are often very scarce (if not absent altogether) due to the challenges inherent in collecting such information. Thus bedload transport dynamics have to be predicted at the basin scale by relying on limited (in space and time) field observations. However, models capable of simulating bedload transport at the network scale in mountain rivers are very few, and to the best of our knowledge, their validation has never been carried out.

The primary objective of this research is to evaluate the performance of the D-CASCADE model – after adapting it to work in Alpine rivers – to simulate bedload transport dynamics at a network scale in the Sulden/Solda river basin (Italian Alps). The Sulden catchment was selected due to the sediment transport monitoring station present at its outlet (130 km2) as well as for the long duration of bedload transport throughout the year due to its nivo-glacial hydrological regime. Since 2014, bedload transport has been continuously monitored in the Sulden River using geophones, which provide high-frequency data on bedload movement and capture temporal variations in bedload transport. To calibrate the geophone signals, regular bedload sampling was conducted. The data obtained from these samples provided detailed insights into the grain size distribution of the transported material at the outlet reach of the modelled network. This empirical information was crucial in fine-tuning the adapted D-CASCADE model and refining existing transport capacity formulas to characterize the connectivity properties of the Sulden network in terms of bedload flux dynamics, path lengths and velocities as well as sediment budgeting of the different reaches.

Preliminary validation of the adapted D-CASCADE model shows a promising agreement between predicted and observed bedload transport rates at the monitoring station. The model demonstrates the potential in reconstructing bedload transport patterns across the entire river network, identifying key sediment sources contributing to the overall sediment flux. Additionally, the model illustrates the spatial and temporal variability in bedload transport, highlighting the complexity of sediment dynamics in Alpine rivers.

How to cite: Pitscheider, F., Argentin, A.-L., Doolaeghe, D., Gianini, M., Repnik, L., Bizzi, S., Lane, S. N., and Comiti, F.: Network-scale modelling of bedload transport in Alpine rivers using D-CASCADE model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5869, https://doi.org/10.5194/egusphere-egu25-5869, 2025.

EGU25-6632 | ECS | PICO | GM2.3

Luminescence imaging of single grains of sand reveals their sediment transport history 

Anna-Maartje de Boer, Stuart G. Pearson, Natascia Pannozzo, Tjitske J. Kooistra, Bram van Prooijen, and Jakob Wallinga

Understanding sediment transport routes is crucial for predicting geomorphic changes driven by natural and anthropogenic processes in coastal and fluvial systems. Sediment tracing methods are vital to gain such understanding, but common sediment tracers are usually limited to following sediment released from a specific point. In our TRacking Ameland Inlet Living lab Sediment (TRAILS) project, we explore the use of natural luminescence signals of minerals to trace nourished sediment grains on an ebb-tidal delta. Towards this, we obtained and analyzed sediment samples from the Dutch Wadden Sea, where a mega-nourishment in the Ameland inlet ebb-tidal delta aims to address the sediment demand of the nearby coast and basin.

Insufficient luminescence signal resetting, e.g. poor bleaching, due to limited light exposure, can serve as a tool for sediment tracing by examining variations in the degree of bleach characteristics of luminescence signals with differing bleaching sensitivities within a single grain. This can inform us about light-exposure of that grain and therefore about sediment transport history, as explored by Reimann et al (2015) for a beach nourishment project at the Dutch coastline. Firstly, we hypothesize that slow-to-bleach signals reveal information about the end-member type: native grains in our ebb-tidal delta will be well-bleached in comparison to nourished grains. Secondly, we hypothesize that fast-to-bleach signals give insight into the transport history of grains: native grains will be more or less fully reset within the dynamic tidal reworking system of the Wadden Sea whilst nourished grains will still inherit part of their original signal. Combining information derived from slow- and fast-to-bleach signals thus provides a promising novel approach for tracing sediment grains in dynamic subaqueous environments, and thereby reveals sediment transport pathways of nourished sand grains.

Luminescence tracing methods rely on quantitative information about the potential and efficiency of subaqueous signal resetting. In a one-day experiment we quantified bleaching potential, that is, the light intensity and spectrum as a function of time, depth and tidal stage, and bleaching efficiency, that is the degree of bleaching of slow- and fast-to-bleach luminescence signals (de Boer et al., 2024a). Strongest subaqueous light attenuation took place during low tide when sediment concentrations are the highest, we also observed stronger attenuation of the ultraviolet part of the light spectrum. Light-sensitive luminescence signals, such as low-temperature feldspar IRSL, bleached more rapidly than less light-sensitive signals, such as high-temperature feldspar post-IR IRSL. None of the investigated signals were fully reset after 13.5 hours of light exposure, even for subaerially exposed samples. We then collected and analyzed over 100 sediment samples from the Ameland ebb-tidal delta. Using an EMCCD camera (de Boer et al., 2024b), we imaged a multitude of single-grain luminescence signals to explore the native or nourished origin of these sand grains. Ultimately, we aim to integrate these findings with Lagrangian sediment transport models to better understand spatial and temporal coastal sediment dynamics and inform coastal nourishment strategies (Pearson et al., 2022).

How to cite: de Boer, A.-M., Pearson, S. G., Pannozzo, N., Kooistra, T. J., van Prooijen, B., and Wallinga, J.: Luminescence imaging of single grains of sand reveals their sediment transport history, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6632, https://doi.org/10.5194/egusphere-egu25-6632, 2025.

EGU25-11090 | PICO | GM2.3

A field-based protocol to approximate variability in critical Shields coarse-bed rivers at the patch scale 

Daniel Vázquez-Tarrío, Estrella Carrero-Carralero, Raúl López, Fanny Ville, Damià Vericat, and Ramon J. Batalla

Predicting the flow conditions required to entrain sediment in gravel-bed rivers is essential for many issues, such as river ecology, flood risk assessment, river restoration and sustainable river management, among many others. In this regard, the critical Shields parameter is the most commonly used metric to characterise particle entrainment in bedload transport studies. Consequently, the determination of critical Shields is fundamental to the prediction of bedload transport in gravel-bed rivers. Conventional field studies have focused on estimating a reach-averaged Shields stress, despite the large spatial variability that this parameter exhibits at the reach scale. This is largely due to the lack of standardised field approaches for characterising Shields stress in a spatially distributed manner. In this work, we propose a field-based procedure for estimating the frequency distribution of critical Shields at the patch scale in a gravel-bed river, based on the measurement of resistance to movement of individual clasts and a number of variables related to the position and orientation of grains. Following this procedure, we have approximated the patch-scale variability of particle entrainment conditions in a gravel bar of the Upper Cinca River, located in the southern watershed of the Pyrenees. The results (mean Shields ~0.03) are consistent with previous estimates of critical Shields in this river and with established theory of particle entrainment in gravel-bed rivers. We believe that this method has great potential to provide valuable field information on particle entrainment.

Ackowledgements: This research benefitted from the methods and outcomes of the MorphHab research project (PID2019-104979RB-I00/AEI/10.13039/501100011033, Ministry of Science, Innovation and Universities (MICINN), Government of Spain). The work by the first author is also part of the 2023–2026 grant signed between the Spanish Directorate General for Water (DGA-MITERD; Government of Spain) and the Spanish National Research Council (CSIC-Ministry of Science, Innovation and Universities), which includes action “Sedimentary Morphodynamics” (20233TE012: IGME-CSIC; Tarquín 2 Project).

How to cite: Vázquez-Tarrío, D., Carrero-Carralero, E., López, R., Ville, F., Vericat, D., and Batalla, R. J.: A field-based protocol to approximate variability in critical Shields coarse-bed rivers at the patch scale, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11090, https://doi.org/10.5194/egusphere-egu25-11090, 2025.

EGU25-11412 | PICO | GM2.3

Exploring Variabilities in Gravel Mobility Using Force-Balance Models 

Edwin Baynes, David Whitfield, Stephen Rice, Richard Jeffries, and Kate Mathers

Understanding the variabilities of bedload mobility is fundamental in predicting the likelihood of erosion and deposition patterns in gravel bedded rivers, which subsequently assist towards modelling geomorphic adjustment and flood risk change over reach to catchment scales. In most applications, the shear stress required to initiate sediment transport (τ*c) is typically assumed from relations with channel slope or the median bed material grain size, and is generally assumed temporally constant. However, flume investigations identify important relations between grain arrangement (for example, grain protrusion and imbrication) and sediment flux, which vary in response to flood history. Given the complexities of river systems, grain-scale linkages between water-working history, bedload characteristics, and grain mobility remain largely unexplored in the field.

 

We use a combination of gravel bed microtopography data, collected via structure-from-motion photogrammetry, and in-situ grain resistance tests to resolve a grain force balance model for 45 upland gravel surfaces across England and Wales. Grain resistance forces (FR), and subsequent estimates of τ*c, are used to explore grain scale drivers of particle mobility, as well as their spatial and temporal variabilities. We interpret flow histories of sampled surfaces using typical water-working indicators (including bed surface roughness, imbrication extent and grain size sorting). Water-working metrics are compared against resistance force distributions, to address the hypothesis that conditioned surfaces exhibit systematically higher mobility thresholds. We also consider the relative role of grain shape on bed topography and stability trends. In practical application, our findings can offer more targeted, process-based, estimates of τ*c for a given channel reach, even when grain surface characteristics are only known qualitatively. Such improvements in τ*c estimates are critical in furthering our ability to predict sediment fluxes and geomorphic change in gravel dominated channels, particularly in response to climate change, where the temporal sensitivity of τ*c is likely to be important.

How to cite: Baynes, E., Whitfield, D., Rice, S., Jeffries, R., and Mathers, K.: Exploring Variabilities in Gravel Mobility Using Force-Balance Models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11412, https://doi.org/10.5194/egusphere-egu25-11412, 2025.

EGU25-11920 | ECS | PICO | GM2.3

Enhancing sediment transport model reliability through Sensitivity Analysis: A Case Study in the Po River 

Sahansila Shrestha, Elisa Bozzolan, Diane Doolaeghe, Nicola Surian, and Simone Bizzi

The limited observational data on river bedload presents a significant challenge in understanding sediment transport processes. However, with recent advancements in computing capability, availability of remotely sensed data, and smart sensors, it is nowadays possible to model these transport processes in river networks at catchment scale. Nevertheless, the results of these models are often not robust due to inherited uncertainty and the stochastic nature of the input parameters. To manage these uncertainties and improve the robustness of model outputs, sensitivity analysis plays a crucial role. Sensitivity analysis is a method to study how changes in a numerical model's input factors contribute to variations in its output.

This project aims to apply Global Sensitivity Analysis (GSA) techniques to the D-CASCADE (Dynamic CAtchment Sediment Connectivity And Delivery) model, for the Po River network in Italy. D-CASCADE is a network-based (or graph-based) model that simulates material movement as distinct transport processes at the reach scale, or ‘cascades,’ defined by their provenance, sediment volume, and interactions downstream, at daily timestep.

To conduct the GSA, we use the SAFE toolbox, supporting both the generation of 5,000 random input factor combinations within defined ranges and distributions, as well as the quantification of the impact of each input factor's variation on the output.

In this work, we focus on the sensitivity estimation of active channel widths and riverbed slopes for every reach of the simulated network. These two input factors are key drivers of the transport capacity and the consequent sediment fluxes generated for the various sediment transport formulas implemented in D-CASCADE. The active transport width (the portion of the channel where bedload transport is active for a specific discharge) is largely unknown, even in data-rich contexts. Hydraulic slopes are also often unknown and generally replaced with topographic slopes which are largely dependent on the quality of the DEM used.  Active widths and slopes are then structurally inherently uncertain although they drive the model results. Through GSA, we evaluate how simultaneous random changes in these two input factors affect the simulated sediment fluxes and budgets. Results are analyzed both at the reach scale (sensitivity to local parameters) and the network scale (sensitivity to upstream parameters).

The presented methodology allows us to obtain important information about the effects of structural uncertainties in sediment transport modelling at network scale. These findings provide a foundation for enhancing the model's accuracy and resolving uncertainty in sediment transport prediction.

How to cite: Shrestha, S., Bozzolan, E., Doolaeghe, D., Surian, N., and Bizzi, S.: Enhancing sediment transport model reliability through Sensitivity Analysis: A Case Study in the Po River, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11920, https://doi.org/10.5194/egusphere-egu25-11920, 2025.

EGU25-12444 | PICO | GM2.3

The impact of cohesive material on gravel entrainment 

Rebecca Hodge, Elowyn Yager, Hal Voepel, Julian Leyland, David Sear, and Danette Sitorus

Predicting when riverbed sediment is mobile is essential for managing the morphology and ecology of gravel-bed river channels. However, our ability to predict critical shear stress (τc) is still such that predictions are only accurate to an order of magnitude at best. One aspect which is often overlooked when predicting grain entrainment, and which likely contributes to our poor predictions of τc, is the role of any cohesive material surrounding the gravel grains. This material could be clay, as is commonly found in gravel-bed rivers draining agricultural catchments, and/or biological, such as produced by caddisfly larvae, mussels and biofilms. To assess the potential impact of non-biological cohesion we parameterise a force-balance grain entrainment model to demonstrate that adding plausible values of cohesion can produce an order of magnitude increase in τc. We compare our results to two sets of field measurements of grain entrainment forces. The first set are from Bury Green Brook, UK, where there is local variation in the amount of clay matrix in the gravel bed and we assess differences in entrainment forces between individual grains. The second set comprises data from multiple sites with varying amounts of fines in the bed and we compare average entrainment forces. Our field data are consistent with the model results, demonstrating the potential importance of accounting for cohesion when predicting τc. Finally, we demonstrate that cohesive forces from clay are also sensitive to water content, and so may be most important in ephemeral channels.

How to cite: Hodge, R., Yager, E., Voepel, H., Leyland, J., Sear, D., and Sitorus, D.: The impact of cohesive material on gravel entrainment, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12444, https://doi.org/10.5194/egusphere-egu25-12444, 2025.

EGU25-12946 | PICO | GM2.3

Multiscale Sediment Connectivity Analysis in Clay-Dominated Lithology  

Federica Fiorucci, Michele Santangelo, and Mauro Rossi

Understanding sediment connectivity is critical for sustainable sediment management. This research focuses on clay-dominated areas of the Northern Apennines, characterized by high landslide activity and sedimentary disequilibrium due to anthropogenic and natural disturbances. These conditions create an ideal testing ground for evaluating sediment transfer processes and restoration strategies. 

The study employs a multiscale approach, integrating high-resolution digital terrain models (DTMs) at 5-meter resolution with detailed DEMs derived from drone-based LiDAR surveys (DJI Matrice 300 and L1 payload). These datasets enable detailed assessments of sediment transfer dynamics, with a focus on the influence of landslides on fluvial systems. 

The SedInConnect model is used to calculate structural sediment connectivity indices, identifying pathways and barriers that influence sediment transfer and highlighting critical areas for intervention. By combining SedInConnect’s spatial analysis of connectivity with LANDPLANER’s temporal modeling of sediment fluxes, the study provides a multidimensional understanding of sediment dynamics. This integration enables the identification of vulnerable areas and the design of targeted management interventions or mitigating erosion in high-risk zones. 

Drone-based LiDAR surveys represent a technological breakthrough, offering high temporal resolution and allowing frequent monitoring of topographic changes. These data are essential for detecting landslide-induced geomorphic changes and refining event-driven sediment dynamics models. By integrating field observations, remote sensing, and advanced modeling, the study delivers a robust and scalable framework for assessing sediment connectivity. 

These advancements offer transformative tools for understanding and managing sediment dynamics, contributing to the development of more resilient and sustainable fluvial systems in clay-dominated landscapes. This approach is particularly valuable for designing and implementing sediment management strategies to mitigate environmental and infrastructural impacts.

How to cite: Fiorucci, F., Santangelo, M., and Rossi, M.: Multiscale Sediment Connectivity Analysis in Clay-Dominated Lithology , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12946, https://doi.org/10.5194/egusphere-egu25-12946, 2025.

Catastrophic sediment release in fluvial systems is largely driven by landsliding that occurs naturally in mountain belts during extreme events, such as earthquakes or storms. Sediments are routed through the river system until they are stored either permanently in alluvial fans and lakes or temporarily in floodplains. The river response to such catastrophic sediment release has already been studied with 2D numerical models using a single effective grain size. Yet, in natural systems, the sediment grain size distribution can span several orders of magnitude and evolves during transport.

The role played by the grain size distribution on morphodynamics depends on transport modes and on grain size interactions. On one hand, fine sediments that tend to be transported in suspension and thus higher in the water column than coarse sediments contribute to floodplain formation and maintenance. On the other hand, coarse sediments that tend to be immobile or transported as bed load contribute to armouring of the channel bed surface that prevents its degradation and in turn leads to channel widening.

Assuming a single effective grain size may limit accurate forecasting of morphodynamic and sedimentological changes in rivers systems during landslide-induced sediment cascades. Modelling the response of a river reach in 3D, meaning that both morphodynamics (2D) and stratigraphy (1D) are resolved may be challenging due to computational time and computer memory. To cope with these limitations, we propose a 2.5D numerical model as a simplified approach. It incorporates: i) a multi-grain size sediment transport model with the ability to capture the transport of suspended and bedload material as well as the dispersion rate and sediment sorting patterns of various grain sizes such as armouring and downstream fining (threshold of motion and explicit grain-size specific entrainment and deposition rates), ii) an explicit transfer of sediment from the river channel to adjacent floodplains (based on the vertical distribution in the water column), iii) freely evolving channel width and slope, and iv) an algorithm to handle channel and floodplain sedimentary records (stratigraphic layers).

We conducted numerical simulations on a constricted river reach that consists of a straight channel with a floodplain on both sides. Numerical simulations reveal: i) how the grain-size specific signals propagate in a river reach and are preserved in the channel and floodplain stratigraphy in response to a catastrophic sediment release, and ii) how the channel width adjusts with stochastic flow conditions and sediment supply.

These preliminary results were obtained in the context of the SCALEES (Signature of sediment CAscades following Landslides triggered by Extreme Events in the Stratigraphy) project funded by the European Union. The combination of empirical data with numerical simulations will allow us to predict for the first time the full signal (all grain sizes) of sediment cascades preserved in stratigraphy in response to an extreme event at the scale of a catchment. It will also pave the way for inverting the stratigraphic record of landslide induced sediment cascades for quantitative insights into their response amplitudes and relaxation times.

How to cite: Le Minor, M., Lague, D., Howarth, J., and Davy, P.: Coupling a channel width evolution model and a multi-grain size sediment transport model: a simplified approach to predict the response of a river reach to a catastrophic sediment release, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14139, https://doi.org/10.5194/egusphere-egu25-14139, 2025.

EGU25-15136 | ECS | PICO | GM2.3

Path Length and Sediment Flux Validation in Braided River Systems: Application of the VMD Method and D-CASCADE Model 

Lindsay Capito, Diane Doolaeghe, Elisa Bozzolan, Nicola Surian, Walter Bertoldi, and Simone Bizzi

The movement of sediment through river networks is crucial for the health and functionality of river ecosystems, flood control, and water availability. Network-scale sediment connectivity models have emerged in recent decades but lack robust validation with field measurements. Here, we perform a path length-based application of the morphological method, the Variational Mode Decomposition (VMD) method, to the Tagliamento River, a large braided river in northeastern Italy, to validate the sediment flux estimates generated by the network scale sediment connectivity model D-CASCADE.

The results indicate that D-CASCADE can generate sediment flux estimates that align with those derived from the VMD method and with values documented in literature. Furthermore, we observe that the generated path length estimates align with the expected path length based on the spacing of confluence-diffluence couplets which has been previously proposed as a proxy for path length. These results underscore the need for careful calibration of grain size distributions for specific rivers to improve model accuracy. Additionally, we identify the importance of estimating a fundamentally unknown input parameter, the active transport width (the part of the river channel where bedload is moving for a specific discharge), and its impact on the modeled sediment transport estimates. Finally, we see from the field acquisitions that even during small flood events on the Tagliamento, there is significant compensation when comparing the erosion and deposition volumes during each flood event.

These results demonstrate that the VMD method provides reasonable estimates of path length and sediment flux, thereby serving as a valuable validation tool for network-scale sediment connectivity models and increasing the robustness of the D-CASCADE model in large, complex river systems. The presented field data also help clarify when topographic changes are not a reliable representation of bedload fluxes due to high flow events or confined planform morphology, which then limits the applicability of the VMD method. Overall, the present study is a step forward in validating and refining our understanding of sediment transport processes in braided river environments and provides practical implications for the sustainable management of riverine ecosystems.

How to cite: Capito, L., Doolaeghe, D., Bozzolan, E., Surian, N., Bertoldi, W., and Bizzi, S.: Path Length and Sediment Flux Validation in Braided River Systems: Application of the VMD Method and D-CASCADE Model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15136, https://doi.org/10.5194/egusphere-egu25-15136, 2025.

EGU25-15661 | ECS | PICO | GM2.3

Estimation of suspended sediment concentration using satellite remote sensing data in Lake Tana, Ethiopia 

Afework Ashagrie Simegn, Girma Worku Awoke, Sofie Annys, Amaury Frankl, and Gert Verstraeten

Soil erosion by water from upland areas results in on-site and offsite problems in the catchment and aquatic ecosystems such as lakes and rivers. As such, up-to-date information on erosion rates and suspended sediment fluxes in rivers is indispensable to manage the impact of soil erosion, sediment transport, and sedimentation. However, detailed spatial and temporal information on erosion and sediment dynamics is rare, as it is labor-intensive and costly to obtain, particularly in developing countries. The advent of satellite remote sensing applications has provided the opportunity to monitor sediment fluxes by assessing the suspended sediment concentration (SSC) of rivers and lakes. This approach may provide a cost-effective alternative to ground-based sampling schemes. However, satellite-based approaches to monitor sediment fluxes require calibration and validation as the relation between SSC and optical properties of the water recorded by satellite sensors may vary with changing sediment properties. 

Here, we used empirical models to estimate SSC values from optical sentinel 2 data for Lake Tana in Ethiopia using in situ collected water samples. Moreover, in situ reflectance data, which were measured using an ASD Field Spec 4 spectroradiometer instrument, from water samples collected at Lake Tana are used as well. SSC and in situ reflectance measurements were conducted for 546 water samples collected from the lake, particularly from the river plumes of the two most important rivers draining to Lake Tana, i.e. Gumara and Giligel Abay.  The sample SSC values ranged from 1.50 mg/L to 4,146 mg/L. The samples were classified into two categories:  low SSC (≤ 250 mg/L) and high SSC (> 250 mg/L), as the optical properties of water are significantly influenced by its constituents. The individual bands in the NIR and visible spectrum exhibited a good correlation (R2 = 0.73, RMSE = 30.69 mg/L) for low SSC-values over Lake Tana. Moreover, the multilinear regression (MLR) analysis using both the visible and NIR bands of low SSC-conditions improved results compared to using individual bands (R2 = 0.84, RMSE = 23.37 mg/L). In contrast, high SSC water samples from Lake Tana did not correlate well with individual bands. However, combining the NIR and red bands generally improved the estimation of SSC for high SSC values (R2 = 0.9, RMSE = 0.26 mg/L).  

The established relations between optical properties and field-based SSC values will be applied to long-term timeseries of optical data to assess the temporal variations in sediment concentration in rivers draining to Lake Tana, and in Lake Tana itself. These timeseries will be compared to optical data on vegetation changes in the catchment to identify hot spots in both space and time that are responsible for elevated fluxes of sediment to Lake Tana. 

How to cite: Ashagrie Simegn, A., Worku Awoke, G., Annys, S., Frankl, A., and Verstraeten, G.: Estimation of suspended sediment concentration using satellite remote sensing data in Lake Tana, Ethiopia, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15661, https://doi.org/10.5194/egusphere-egu25-15661, 2025.

EGU25-16407 | ECS | PICO | GM2.3

PhotoMOB: a GIS tool to monitor spatial and temporal bed mobility at the patch scale 

Fanny Ville, Damià Vericat, Colin Rennie, and Ramon J. Batalla

The stability or, conversely, the mobilisation of riverbeds varies in time and space, making it a complex phenomenon to study. The size and intensity of mobile grains can lead to disturbance of the substrate that supports physical habitats and can therefore control the presence of aquatic organisms. The degree of mobility of a given grain size fraction (GSF) can be approximated by assessing the proportion of its grains that are mobile. On the other hand, the relative degree of mobility can be expressed as the ratio between the proportion pi of this fraction among all mobilised grains compared to its initial proportion at the surface of the bed Fi. A condition of full mobility is reached when the fraction's proportion among the mobilised grains is equal to or greater than its initial proportion at the surface (pi /Fi≥ 1). An underrepresented fraction is said to be partially mobile (pi /Fi<1).

We present PhotoMOB, a GIS-based tool to characterise (i) grain shape (i.e. axis size, orientation, roundness, compactness, elongation), (ii) patch organisation (i.e. proportion of fine material cover, proportion of overlapping grains) and (iii) mobility magnitude of gravel river beds from repeated digital photographs taken before and after targeted hydrological events. It is based on the detection and the comparison of the shape of grains identified at the same coordinates (location). PhotoMOB allows identification of coincident grains (immobile) and new grains (mobile). Several variables can be extracted from this categorisation, such as: the overall proportion of mobile or immobile grains (in number or surface area), the maximum mobile or immobile diameters, the proportion per individual GSF of grains that remain immobile (stable) and newly identified grains. In addition, changes in fine material cover, grain overlap can be assessed and the percentiles of the surface grain shape distribution before and after a targeted hydrological event, as well as the distribution of exclusively immobile and/or mobilised grains, can be calculated.

Automatic classification applied to perfect (manual) digitisation of grains gives mean absolute errors for fractional mobility estimation of less than 3%, while automatic classification applied to automated digitisation with 10 minutes of manual grain boundary revision gives errors of around 8%. This approach has been developed, tested and applied in gravel-bed mountain rivers affected by hydropeaking, which induces partial mobility.

 

Ackowledgements: This work is carried out in the background of the projects MorphHab PID2019-104979RB-I00 / AEI / 10.13039/501100011033) and Undammed TED2021-130815B-C31 / MCIN/AEI/10.13039/501100011033, funded by the Spanish Ministry of Science, Innovation and Universities and the EU “NextGenerationEU”/PRTR. All authors are part of the Fluvial Dynamics Research Group –RIUS, a consolidated group recognized by the Generalitat de Catalunya (2021 SGR 01114). 

How to cite: Ville, F., Vericat, D., Rennie, C., and Batalla, R. J.: PhotoMOB: a GIS tool to monitor spatial and temporal bed mobility at the patch scale, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16407, https://doi.org/10.5194/egusphere-egu25-16407, 2025.

EGU25-18605 | ECS | PICO | GM2.3

Suspended sediment measurements by hydro-acoustic multi-frequency echosounders 

Jakob Höllrigl, Koen Blanckaert, David Hurther, Guillaume Fromant, and Florian R. Storck

The suspended sediment concentration (SSC) in rivers is commonly indirectly estimated from optical turbidity measurements in one single point. Calibration based on regular sampling and laboratory analysis allows converting the optical turbidity into SSC. The regular sampling and laboratory analysis are time-consuming and expensive.

A hydro-acoustic multi-frequency approach has advantages as an alternative to optical turbidity measurements. Backscatter data collected with hydro-acoustic echosounders contains information on the suspended particles along an entire profile. The conversion of backscatter into SSCs from an acoustic single-frequency system, like most standard ADCPs are, requires knowledge on the characteristics of the suspended particles, in particular on their average size and the grain size distribution. These characteristics can be estimated by analysing water samples in the laboratory.

The present contribution reports measurements of the SSC along an entire profile with a multi-frequency system. The multi-frequency approach allows estimating the particle characteristics from the backscatter data. Hence, the conversion of backscatter into SSC does not require water samples and laboratory analysis anymore. The potential of the hydro-acoustic multi-frequency approach is illustrated with in-situ river measurements and laboratory experiments that cover a broad range of sediment concentrations and sediment characteristics.

How to cite: Höllrigl, J., Blanckaert, K., Hurther, D., Fromant, G., and Storck, F. R.: Suspended sediment measurements by hydro-acoustic multi-frequency echosounders, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18605, https://doi.org/10.5194/egusphere-egu25-18605, 2025.

Sediment transport plays a crucial role in shaping our natural and engineered landscapes, affecting everything from riverbanks to coastal regions and ecological habitats. It is key to effective disaster management, helping predict and mitigate the effects of floods, landslides, and coastal erosion. However, modeling how sediment moves through water and landscapes remains a complex challenge. This complexity is due to the unpredictable nature of turbulent flows and sediment movement, compounded by issues such as natural variability, lack of sufficient data for accurate model testing, and high computational demand.

This research introduces an innovative approach by integrating Lagrangian turbulent velocity theory into sediment transport models. By developing a new model that utilizes differentiable stochastic processes, this study aims to enhance our ability to predict and understand how particles behave in turbulent flows. This advanced modeling technique addresses key challenges like the unpredictability, intermittent behavior, and memory effects associated with particle movement in turbulent conditions. Ultimately, this research seeks to refine our understanding of sediment dynamics, pushing the boundaries of existing models and providing more reliable tools for environmental management.

How to cite: Tsai, C.: Lagrangian Stochastic Sediment Dynamics in Turbulent Flows, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19574, https://doi.org/10.5194/egusphere-egu25-19574, 2025.

Lateritic landscapes are structurally complex systems formed through intense chemical weathering under tropical paleoclimates. These profiles are found in stable, low-relief landscapes across tropical, subtropical, and Mediterranean climates, particularly between 35°N to 35°S. Their vertical structure reflects long-term shifts in climatic, hydrological, and tectonic conditions, offering a valuable "memory" of past environmental changes. Despite their environmental and economic significance, lateritic landscapes remain underrepresented in CZ research, a bias compounded by the concentration of Critical Zone Observatories in the Northern Hemisphere, where shallow, truncated profiles prevail due to glacial erosion. This underrepresentation limits our understanding of long-term CZ processes and how they have shaped subsurface architecture.

This study investigates the subsurface architecture of a lateritic hillslope at the Avon River Critical Zone Observatory (AR-CZO) in Western Australia. Prolonged subaerial weathering since the Cretaceous, followed by mid-Miocene aridification, has created a stratigraphically complex regolith hillslope shaped by weathering, erosion, and colluvial deposition. To resolve the structural complexity of this hillslope, we applied a multi-method geophysical approach, combining electrical resistivity tomography (ERT), horizontal-to-vertical spectral ratio (HVSR) passive seismic methods, and borehole observations. ERT captured fine-scale stratigraphy, delineating the pallid zone, saprolite, and duricrust, while HVSR resolved broader interfaces, such as the duricrust-bedrock boundary and the base of the colluvial deposit.

The results reveal how landscape position influences CZ structure. The hilltop is capped by a duricrust that transitions downslope into an erosional surface, where the pallid zone of the lateritic weathering profile is exposed at the surface. At the foot slope, approximately 11 m of colluvial sediment has accumulated from the erosion of the hillslope material. Bedrock depth estimates differed between methods, with ERT indicating depths of 23 m on the slope and 32 m at the foot slope, while HVSR revealed deeper depths of 31 m and 39 m, respectively. The discrepancy highlights the limitations of ERT in saline environments, where conductivity masks key interfaces, while HVSR’s broader resolution provides more reliable bedrock detection in such conditions. Together, these methods reveal a laterally variable weathering profile that responds to shifts in landscape position, erosion, and deposition.

The complementarity of ERT and HVSR underscores the value of a multi-method geophysical approach for resolving the structural complexity of lateritic CZs. Our conceptual model demonstrates how weathering, erosion, and colluvial processes shape the structure of a deeply weathered hillslope, while also providing a transferable framework for characterizing saline, regolith-dominated systems. Given their depth, age, and capacity to preserve past climatic and tectonic conditions, lateritic CZs offer a vital opportunity to enhance global understanding of long-term CZ evolution. This research addresses the Northern Hemisphere bias in CZ science, highlights the underexplored role of stable, deeply weathered landscapes, and underscores the need for future comparative studies to understand the drivers of heterogeneity in subsurface architecture across CZs worldwide.

How to cite: Weller, J., Jakica, S., Thompson, S., and Leopold, M.: Combining electrical resistivity tomography and passive seismic to characterise the subsurface architecture of a deeply weathered lateritic hill within the Avon River Critical Zone Observatory, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1401, https://doi.org/10.5194/egusphere-egu25-1401, 2025.

The ground substrate is a new concept in the field of natural resources proposed by Chinese scientists in 2020 (Ministry of Natural Resources, 2020). It is the basic material that supports and nurtures various natural resources such as soil, forests, grasslands, wetlands, and water. The layer of ground substrate is the most active geological space for the exchange of substances and energy such as water, heat, salt, gas, carbon, etc. It is also serving as a bridge link between the land cover layer and the underground resource layer. The proposal on concept of ground substrate has clarified new directions and goals for geological survey to support ecological civilization construction and natural resource management, has great significance.

In different climate zones such as humid, semi humid, semi-arid, and arid in China, there are significant differences in the material composition, genetic types, and characteristic physicochemical properties of ground substrates, which call ground substrate heterogeneity by us. In recent years, based on multiple ground substrate surveys and research projects, some important conclusions has been gained. The first is we revealed the constraint mechanisms of the physical structure, mineral element composition, and chemical properties of ground substrates on the types, NDVI, NPP of vegetation ecology in the key ecological functional areas in northern China and hilly mountainous areas in southern China. The second is the determination of the bottom boundary of the ground substrate layer requires comprehensive consideration of five factors: they are depth of the underground variable temperate zone, the roots depth of crop and vegetation, the depth of the surface karst development zone, the thickness of the weathering crust, and the burial depth of the groundwater level. It is generally believed that the depth of the ground substrate layer is less than 20 meters. The third is the key constraint layer of ground substrate (rock and soil layers that have important control and influence on vegetation and crop growth, water and salt storage and transport, etc.) is a special layer that should be given special attention in ground substrate filed survey.

More detailed about the scientific connotation and theoretical framework of ground substrate, please see the published paper(Hao Aibing, Yin Zhiqiang*, Li Hongyu, Lu Qinyuan, Peng Ling, Shao Hai, Jiang Qida, Zhao Xiaofeng, Liu Jiufeng, Pang Jumei, Yang Ke, Chen Peng, Kong Fanpeng, Hou Hongxin, Lu Min. 2024. The scientific connotation and theoretical framework of ground substrate. Acta Geologica Sinica. 98(11):3225-3237)

How to cite: yin, Z., peng, L., and hao, A.: The concept of ground substrate and its physical structure & mineral element composition constrain mechanisms on vegetation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1441, https://doi.org/10.5194/egusphere-egu25-1441, 2025.

EGU25-1952 | ECS | Orals | HS8.2.8

Clogging model of hyporheic exchange based on coupled lattice Boltzmann discrete element simulations 

Xudong Zhang, Atsushi Takai, Tomohiro Kato, and Takeshi Katsumi

The hyporheic exchange between the surface water and the underground water is considered a significant process in the natural water cycle system. Some sediment particles in the riverbed can be carried to the exchange channel under the stream effect. Over time, these particles accumulate on the channel can decrease the exchange efficiency of water resources, and induce clogs. The clogging problem of the exchange channel may further induce various geological and environmental disasters such as the shrinkage of lakes and desertification.

To detail the clogging mechanism in the exchange channel, we simulated the exchange clogging process on the exchange channel based on a coupled lattice Boltzmann method (LBM) and discrete element method (DEM). The results indicated particles could form an arch structure clogging the channel orifice. The formation of the clogging arch prevented the discharge of soil particles and greatly decreased the fluid velocity. Notably, the fluid velocity distribution around the orifice is in a certain shape according to the velocity of the LBM cells—the size of the shape regularly changes with the distance to the channel orifice. The variation of the average fluid velocity in the orifice first increases to a peak (about 0.497 cm/s) in the initial time and then decreases to an approximate value after clogging (about 0.037 cm/s). The maximum velocity is almost thirteen times the minimum, indicating that the clogging effect can reduce the water velocity of hyporheic exchange by more than one order of magnitude. In addition, it was found that the soil skeleton was necessary for forming clogs in polydisperse particle systems by analyzing the clogging arch-forming process. The sediment particles in different scales have different effects on the clogging arch. The large particles in the sediments are closely related to the formation of the soil skeleton. The fine particles were involved in the filling and enhancing of the soil skeleton.

Based on our simulation analysis, an explanation for the clogging formation under microscopic conditions was proposed, leading to a detailed description of the exchange clogging in the hyporheic exchange channel. In addition, some mechanism statements to better understand the exchange phenomenon in the water cycling ecosystem are also provided.

How to cite: Zhang, X., Takai, A., Kato, T., and Katsumi, T.: Clogging model of hyporheic exchange based on coupled lattice Boltzmann discrete element simulations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1952, https://doi.org/10.5194/egusphere-egu25-1952, 2025.

EGU25-2490 | Orals | HS8.2.8

Spring and stream intermittency in an instrumented steep Himalayan Mountain catchment 

John Armitage, Kapiolani Teagai, Niels Hovius, Luc Illien, and Christoff Andermann

The pathway for rainfall into stream flow in mountain catchments can be fast via surface run-off or short-lived storage in the weathered zone, or slow via the deep fractured bedrock groundwater system. In mountainous topography, springs can be found at almost all elevations, suggesting that groundwater storage occurs at all elevations. There is however uncertainty as if this storage is short lived, confined to the weathered zone, or longer lived and is part of the groundwater system. Intermittent streams and springs might reflect the storage of water within the subsurface. To measure stream intermittency and the migration of the associated headwater springs we installed intermittency loggers based on repurposed HOBO luminosity loggers along five gulleys within the Kahule Khola catchment in central Nepal.

The intermittency loggers measure an electric current when the circuit is closed by surface moisture and flowing water. The loggers were installed in spring 2023 before the pre-monsoon and were removed in November 2024. At low elevation, three series of loggers were installed in gullies below the village of Listi. These below Listi loggers had perennial springs at their lowest elevation. Furthermore, one series of loggers ended at an ERT repeat survey that showed evidence of year-round shallow subsurface saturation. At high elevation, two series of loggers were installed near the village of Bagham, below an open meadow where ephemeral springs were mapped (we call these the meadow loggers). A coincident ERT repeat survey showed evidence of lateral flow of groundwater within this region.

The loggers recorded three distinct phases: (1) The pre-monsoon, where individual storm events can be registered along each gulley as separate wetting events. (2) Monsoon, where there is a continuous and high conductivity measurement for all loggers, representing continuous flow of surface water. (3) The dry season, which starts with a recession in the electric current observed, followed by sparce wet events. The below Listi systems dried completely within the dry season, while the meadow gulleys recorded low but non-zero electric currents even throughout the dry season. The loggers did not record any evidence of spring migration down the gulleys, rather a uniform drying after rainfall events at all locations, with prolonged wetness post monsoon only seen for loggers that were situated just above known perennial springs. The observations would therefore suggest that intermittent run-off comes from the temporary storage in the weathered zone that dries out at the same rate across the catchment, while persistent flow is from points where the topography intersects with the deeper groundwater reservoir. Run-off within the steep catchment therefore operates through two coexisting systems, (1) an intermittent system that is fed from temporary storage of water in the weathered zone, where there is no distinct headwater spring, and (2) perennial streams fed by groundwater springs.

How to cite: Armitage, J., Teagai, K., Hovius, N., Illien, L., and Andermann, C.: Spring and stream intermittency in an instrumented steep Himalayan Mountain catchment, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2490, https://doi.org/10.5194/egusphere-egu25-2490, 2025.

EGU25-2917 | Posters on site | HS8.2.8

Accelerating Critical Zone Science with an International Network of Networks 

Jeffrey Munroe, Bhavna Arora, Kevin Bishop, Theresa Blume, Heye Bogena, Elizabeth Boyer, Isabelle Braud, Jérôme Gaillardet, Ralf Kiese, and Steffen Zacharias

The international Critical Zone Network of Networks (CZ-NoN) project, launched in January 2025 and funded by the US National Science Foundation, promotes the study of the Earth’s Critical Zone (CZ), the vital near-surface environment where essential life-supporting processes converge.  Building on previous investments in CZ research, CZ-NoN fosters collaboration and communication between existing and emerging environmental observatories and monitoring networks worldwide.  By establishing a unified framework for collaboration and discussion, CZ-NoN addresses long-standing challenges such as fragmented methodologies, redundancies, poor communication, and barriers to data discoverability and accessibility.  Key project components include planning meetings, workshops, and an online webinar series aimed at building community, showcasing new efforts, and increasing awareness of ongoing CZ research.  In parallel, a global polling effort will compile a crowdsourced list of grand research questions to guide future CZ studies.  By bringing together researchers from different countries and disciplines, and prioritizing cooperation over competition, CZ-NoN will accelerate scientific research and position the international research community for future funding opportunities to support complex, integrated study of the global CZ across diverse socio-environmental conditions.

How to cite: Munroe, J., Arora, B., Bishop, K., Blume, T., Bogena, H., Boyer, E., Braud, I., Gaillardet, J., Kiese, R., and Zacharias, S.: Accelerating Critical Zone Science with an International Network of Networks, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2917, https://doi.org/10.5194/egusphere-egu25-2917, 2025.

Tropical vegetation plays a vital role in global ecosystem services, with one critical aspect lying in its hydrological functions of water cycle regulation. Climate change and accelerated human interventions threaten the stability of tropical vegetation, associated with profoundly hydrological changes particularly in recent decades. Despite various studies on land-atmosphere feedback using earth system models, the regulation of terrestrial hydrological components remains unclear over tropical regions, due primarily to inherent limitations of models in accurately simulating terrestrial water storage (TWS) and runoff. Here, we combine multisource observations to reveal a disparity pattern in storage-runoff interactions over tropical regions for the past two decades. Using satellite-based Landsat optical archives, Global Ecosystem Dynamics Investigation, GRACE gravimetry, and gauge-based runoff database, we show that large-scale forest degradation and cropland expansion have weakened moisture recycling over the eastern tropical South America and eastern tropical Africa (Region I), indicated by a significant decrease in net precipitation input (precipitation minus evapotranspiration). This further causes declines in both TWS and streamflow, shown as a pattern of “less storage and less runoff” due to vegetation degradation. In contrast, over the western tropical South America, western tropical Africa, and tropical Asia (Region II), we did not find marked changes in land cover but a significant increasing trend in vegetation greenness and leaf area index. This is associated with a significant increase in net precipitation input and an enhanced moisture recycling. The increased water input over Region II causes an increase in TWS but a decline in streamflow, shown as a pattern of “more storage but less runoff” due to the decrease in rainfall-runoff generation induced by vegetation growth. The disparity patterns between Region I and Region II highlight different responses of tropical terrestrial water system to a changing environment. Unlike most past studies relying on land surface or earth system models, this study leverages strengths in advanced observation techniques to explore different mechanisms underlying changes in the tropical terrestrial water system. Findings from this study provide valuable supplements to the current model-based analysis, and inform adaptive strategies for changes over tropical regions.

How to cite: Li, X. and Peng, J.: Multisource observations reveal different roles of tropical vegetation in terrestrial water regulation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7653, https://doi.org/10.5194/egusphere-egu25-7653, 2025.

EGU25-9089 | Posters on site | HS8.2.8

Monitoring the triple oxygen isotope composition of water and biogenic silica at the soil-plant-atmosphere interface: benefits for investigating West African present and past water cycles 

Anne Alexandre, Clément Outrequin, Christine Vallet-Coulomb, Christophe peugeot, Manuela Grippa, Julie Aleman, Claudia Voigt, Amaelle landais, Eric mougin, Ousmane Ndiaye, Corinne Sonzogni, David Au Yang, Jean-Charles Mazur, Martine Couapel, Jérome Ogée, Theodore Ouani, Simon Afouda, Nogmana Soumaguel, Torbern Tagesson, and Rasmus Fensholt

Quantitative data are needed to constrain vegetation-hydroclimate in water cycle modelling. Here, we use the triple oxygen isotope composition (δ'18O and 17O-excess) of water compartments to track water transfers and mixing within the soil-plant-atmosphere continuum. At three AMMA-CATCH sites in Benin and Senegal we monitored the δ'18O and 17O-excess of precipitation, groundwater, soil water and plant water, as well as the 17O-excess of phytoliths, an indicator of atmospheric relative humidity. We found that : 1) the 17O-excess in precipitation is very stable over several years; 2) groundwater has δ'18O and 17O-excess values consistent with a multi-year recharge by modern precipitation; 3) the 17O-excess in soil water shows a limited contribution of evaporated water, despite high evaporation conditions, which has important implications for our knowledge of water transfers within soils; 4) extrapolating linear relationships between δ'18O and excess 17O-excess of leaf and stem water allows us to determine the origin of the water absorbed by the roots. At the savanna and dry forest sites, during the rainy season, grasses absorb soil water supplied by precipitation. In contrast, during the dry season, trees reach the perennial groundwater recharge. 5) the 17O-excess of grass and tree leaf water follow the dynamics of relative humidity; 6) the 17O-excess of grass phytoliths records daily relative humidity during the growing season. These results provide a solid basis for using the triple oxygen isotope composition of water and phytoliths to trace present and past water cycles at the soil-plant-atmosphere interface.

This study was conducted in the framework of the HUMI-17 and PAST-17 projects supported by the ANR (ANR-17-CE01-0002-01 and ANR-22-CE01-0027-01), JA and CV have benefited from a Marie Sklodowska-Curie grant from the European Union (n°101063961 for JA and 101063961 for CV). TT acknowledge funds from FORMAS (Dnr 2021-00644), and the European Union under the Development Smart Innovation through Research in Agriculture (DeSIRA) Initiative (FOOD/2019/410-169).

How to cite: Alexandre, A., Outrequin, C., Vallet-Coulomb, C., peugeot, C., Grippa, M., Aleman, J., Voigt, C., landais, A., mougin, E., Ndiaye, O., Sonzogni, C., Au Yang, D., Mazur, J.-C., Couapel, M., Ogée, J., Ouani, T., Afouda, S., Soumaguel, N., Tagesson, T., and Fensholt, R.: Monitoring the triple oxygen isotope composition of water and biogenic silica at the soil-plant-atmosphere interface: benefits for investigating West African present and past water cycles, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9089, https://doi.org/10.5194/egusphere-egu25-9089, 2025.

The Bassée Observatory, located in the heart of the Seine catchment and part of the Zone Atelier Seine network, is an essential research platform for understanding the hydrological processes associated with the strategic challenges of sustainable water resource management. It focuses on the behaviour of the alluvial plain as a complex and anthropised hydrosystem, considering its long-term geohistorical evolution. Through an extensive network of surface water and groundwater monitoring stations, the observatory highlights the central role of groundwater and its interactions with surface water in the current dynamics of this region. We introduce the new groundwater model of the Bassée, developed as a tool combining the CaWaQS hydrogeological platform with the groundwater utilities of the PEST parameter estimation approach. This integration improves the representation of the heterogeneity of the alluvial plain and provides a solid basis for quantitative decision making. The model is designed to assist stakeholders in addressing the challenges of operating and conserving the alluvial plain in the context of a changing environment.

How to cite: Jost, A., Saias, C., and Renaud, A.: Groundwater modelling in the Bassée alluvial plain: A tool for understanding the dynamics of a complex socio-hydrosystem, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9355, https://doi.org/10.5194/egusphere-egu25-9355, 2025.

EGU25-10061 | ECS | Posters on site | HS8.2.8

Quantifying hydrogeological drivers influencing daily fluctuations in shallow groundwater levels within an altiplanic pristine catchment in Chile. 

Amanda Peña-Echeverría, Cristina Contreras, Jorge Renaud, Sarah Leray, and Francisco Suárez

Daily fluctuations in shallow groundwater levels provide valuable insights into hydro-ecological dynamics and aquifer hydraulic properties. These fluctuations usually depend on hydrological/hydrogeological processes, such as precipitation, evaporation, snow/ice melting/thawing, as well as soil characteristics that influence aquifer response times. The Salar del Huasco basin (20.2°S, 68.8°W; 4,164 m a.s.l.; 1,470 km2) is an endorheic system located in the arid Chilean Altiplano, hosting wetlands and a saline lagoon that sustain part of the region essential biodiversity such as chilean, andean, parina and chica’s flamingos, and it serves as a refuge for migratory birds (e.g., peregrine falcon, golden plover and baird's sandpiper). The area experiences extreme thermal oscillations (4–14°C daily averages; winter lows of -20°C), high potential evaporation (1,200 mm/year), and variable summer precipitation (11–400 mm/year). To explore shallow groundwater dynamics, we monitored for ~1 year two sites near the basin’s salt flat: the north and the south sites. Meteorological, soil, and groundwater levels data were collected at 30-min intervals. At the northern site, daily groundwater level fluctuations ranged from 6 to 45 mm, with a sharp and abrupt 300 mm rise in austral spring. In contrast, the southern site showed daily groundwater level fluctuations between 7 and 58 mm, with multiple rises during winter, ranging from 100 to 300 mm. Distinct patterns emerged at these sites: in the northern site, the maximum diurnal fluctuations correlated with solar radiation, while the southern site showed a more stable behavior, with no clear daily peaks. We applied a water balance to determine how the amplitude of possible input and output fluxes in the system altered the daily level fluctuations, and whether, despite the proximity of both sites (~9 km), soil texture, vegetation cover, and local meteorological-hydrogeological conditions explain the differences in groundwater level behavior.

How to cite: Peña-Echeverría, A., Contreras, C., Renaud, J., Leray, S., and Suárez, F.: Quantifying hydrogeological drivers influencing daily fluctuations in shallow groundwater levels within an altiplanic pristine catchment in Chile., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10061, https://doi.org/10.5194/egusphere-egu25-10061, 2025.

In times of climatic unpredictability driven by a quickly changing climate, it is critical to investigate hydrological processes and water availability in different climatic and geomorphological contexts. Mountains have long been acknowledged as fundamental sources of abundant high-quality water for the densely populated downstream areas. The large volumes of water stored in mountain lakes, reservoirs, and snow caps are extremely important to buffer precipitation variability and sustain ecological and anthropic water uses during droughts. So far, the flow and storage of water in the deeply fractured rock formations constituting the core of mountain massifs have mostly been neglected, even for the long-term water balance. However, recent experimental evidence has shown that poorly porous and conductive fractured bedrock can host aquifers whose contribution to streamflow can be substantial, particularly during droughts.

This study systematically assesses, under a wide range of geomorphoclimatic conditions, how deep subsurface storage and flows affect critical hydrological and hydrogeological variables such as the age of streamflow (as opposed to the age of baseflow), surface seepage, and permanent drainage density. These critical hydrological processes are investigated via a large set of steady-state numerical experiments by modulating surface topography, groundwater recharge, and hydrogeological properties of the subsurface (e.g., formation depth, hydraulic conductivity, and its heterogeneity).

The results quantitatively show, for example, how different morphological and hydrogeological conditions may respond to climate change and can be useful in identifying vulnerable areas where mitigation strategies should be prioritized to cope with water shortages. The study can also help understand where ecological alterations driven by the lack of water can have a more profound impact on riverine habitats and where to expect the shift of species in the future.  

How to cite: Bellin, A. and Betterle, A.: Assessing the Impact of Deep Subsurface Storage and Flows on Hydrological Processes and Water Availability in Mountainous Regions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11743, https://doi.org/10.5194/egusphere-egu25-11743, 2025.

EGU25-12719 | Orals | HS8.2.8

 Infiltration depth, rooting depth, and regolith flushing—A global perspective 

Gonzalo Miguez-Macho and Ying Fan

How deep does the rain regularly infiltrate into the ground? Do plant roots follow? How much infiltration is pumped back to the atmosphere (short-circuiting)  and how much passes below plant roots reaching the water table, flushing the regolith, recharging aquifers and rivers, and eventually reaching the ocean (long-circuiting) thus regulating global biogeochemical cycles and long-term climate? What is the depth that supplies evapotranspiration, and what is the regolith flush rate? What are the implications to global material and energy cycles? The answers depend on local climate–terrain–vegetation combinations. We use observations and high resolution numerical modeling at the global scale to shed light on multiscale causes–feedbacks among climate, drainage, substrate, and plant biomass that interactively create a global structure in the depths and rates of hydrologic plumbing of the Earth's critical zone, informing global models on critical depths and processes to include in Earth-system predictions.

How to cite: Miguez-Macho, G. and Fan, Y.:  Infiltration depth, rooting depth, and regolith flushing—A global perspective, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12719, https://doi.org/10.5194/egusphere-egu25-12719, 2025.

EGU25-12772 | Orals | HS8.2.8

Groundwater controls on headwater stream dynamics 

Clément Roques, Ronan Abhervé, Etienne Marti, Ronny Figueroa, Nicolas Cornette, Alexandre Gauvain, Jean-Raynald de Dreuzy, Sarah Leray, Camille Bouchez, Alexandre Boisson, Luc Aquilina, and Philip Brunner

Headwater catchments, defined as the uppermost segments of drainage networks with intermittent and/or perennial third-order streams, are vital sources of freshwater and nutrients for downstream river basins. Despite their critical role in sustaining natural ecosystems and supporting human services, these systems remain poorly understood and are often referred to as 'aqua incognita1.' A key challenge lies in unraveling the hidden groundwater processes that contribute to storage-discharge dynamics. Recent advances in both in-situ and remote monitoring, combined with innovative modeling techniques, now offer opportunities to capture the complex interactions between surface and subsurface processes across diverse climatic, topographic, and geological contexts.

In this presentation, we will present recent findings from field investigations conducted in headwater observatories, complemented by numerical modeling experiments designed to evaluate the controls of key geomorphic factors on groundwater-surface water interactions. The presentation will explore how landforms, lithologies, subsurface stress, and faults shape hydrological behaviors, including stream baseflow recession, groundwater seepage distribution, flow intermittency, and water residence times. Additionally, we will highlight advances in numerical modeling techniques, particularly through the HydroModPy community modelling platform2, which enhance the representation and calibration of groundwater processes in catchment-scale hydrological models. Through the application of these models on pilot sites, we will illustrate how subsurface heterogeneity influences the predictions of water availability under future climate change scenarios, emphasizing the importance of integrating hydrogeological insights for supporting resilient water resource management.

1 Bishop, K., Buffam, I., Erlandsson, M., Fölster, J., Laudon, H., Seibert, J., Temnerud, J., 2008. Aqua Incognita: the unknown headwaters. Hydrological Processes 22, 1239–1242. https://doi.org/10.1002/hyp.7049

2 Gauvain, A., Abhervé, R., Coche, A., Le Mesnil, M., Roques, C., Bouchez, C., Marçais, J., Leray, S., Marti, E., Figueroa, R., Bresciani, E., Vautier, C., Boivin, B., Sallou, J., Bourcier, J., Combemale, B., Brunner, P., Longuevergne, L., Aquilina, L., and de Dreuzy, J.-R.: HydroModPy: A Python toolbox for deploying catchment-scale shallow groundwater models , EGUsphere [preprint], https://doi.org/10.5194/egusphere-2024-3962, 2025.

How to cite: Roques, C., Abhervé, R., Marti, E., Figueroa, R., Cornette, N., Gauvain, A., de Dreuzy, J.-R., Leray, S., Bouchez, C., Boisson, A., Aquilina, L., and Brunner, P.: Groundwater controls on headwater stream dynamics, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12772, https://doi.org/10.5194/egusphere-egu25-12772, 2025.

EGU25-12792 | ECS | Orals | HS8.2.8

Deep flow behavior and the critical zone in a deep well: A hydrogeological study in Mexico City 

Zaida Martínez Casas, Eric Morales Casique, Selene Olea Olea, and Jose Luis Lezama Campos

In Mexico City, where population growth has significantly increased water demand, a well was drilled to a vertical depth of 1992 meters. 
To understand the groundwater dynamic in the critical zone- an area extending from the surface to the base of the groundwater system, where complex interactions occur between the atmosphere, lithosphere, hydrosphere, and biosphere- various tools were employed, including geophysical log analysis, pumping tests, and groundwater sampling for hydrochemical and isotopic (stable and radioactive) analyses.

The results revealed consistent ion concentrations during hydrogeochemical monitoring, classifying the water as sodium-chloride type with minor nitrate contamination attributed to the use of drilling mud.

Isotopic analysis indicated that the water likely originated from precipitation infiltrating at approximately 3000 meters above sea level, possibly from nearby mountain ranges. Radiocarbon dating estimated a residence time of 2840 years, although additional testing is necessary for confirmation.

Hydraulic tests determined a transmissivity of 768 m²/day and a specific storage of 3.11 × 10⁻⁶ m⁻¹, corresponding to an average hydraulic conductivity of 0.885 m/day. This is a complex hydrogeological system characterized by deep, highly fractured saturated zones. Groundwater in this well originates from the deep infiltration of rainfall in the surrounding sierras, circulating through fractures in volcanic rocks. Initially, the water quality showed temporary mixing with surface water due to the interaction between formation water and drilling mud; however, it later exhibited a distinct chemical composition.

The residence time of the water indicates a dynamic system with varying water ages. The results suggest hydraulic connectivity between different hydrogeological units and an endorheic behavior of groundwater flow in the area. In summary, this study enhances the understanding of groundwater flows in Mexico City, emphasizing the critical zone's role in shaping subsurface processes and highlighting the importance of considering the complexity of these systems for sustainable management.

How to cite: Martínez Casas, Z., Morales Casique, E., Olea Olea, S., and Lezama Campos, J. L.: Deep flow behavior and the critical zone in a deep well: A hydrogeological study in Mexico City, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12792, https://doi.org/10.5194/egusphere-egu25-12792, 2025.

EGU25-13922 | Orals | HS8.2.8

A Scale-Adaptive Framework for Modeling Critical Zone Processes and River Water Quality in the East River Watershed 

Dipankar Dwivedi, Ilhan Özgen Xian, Bhavna Arora, Boris Faybishenko, Michelle Newcomer, Patricia Fox, Carl Steefel, Kenneth Williams, Peter Nico, Susan Hubbard, and Eoin Brodie

Critical Zone processes encompass interactions among rock, soil, water, air, and living organisms, essential for quantifying water and nutrient fluxes and predicting downstream river water quality. High-fidelity reactive transport models (RTMs) are important for understanding Critical Zone processes but are typically computationally expensive, which limits their applicability across large catchments. To address these challenges, we developed a scale-adaptive reactive transport simulation framework that balances process fidelity with computational efficiency. We developed the RiverFlotran Module, which employs fully dynamic 1D shallow-water equations for river hydrodynamics, and integrated it into PFLOTRAN, a subsurface reactive transport model. This integration enables us to simulate bidirectional exchanges at the land-water interface. Subsequently, we developed a machine learning-based exchange function, trained on the simulated data, and tailored for the East River. This function allows us to predict river water quality along the river continuum. This framework was applied to the East River Mountainous Watershed in Colorado, a study site of Berkeley Lab's Watershed Function Scientific Focus Area, to demonstrate its effectiveness in capturing intricate Critical Zone interactions and predicting downstream river water quality. Our study of the East River Floodplain's alluvial aquifer revealed that prevailing anoxic conditions generate pronounced redox gradients, resulting in the downstream export of dissolved iron and nitrogen near meander bends. These bends consistently serve as nitrogen hotspots, irrespective of water levels, driven by variations in river stage, bathymetry, and meander geometry, such as sinuosity. This modeling framework provides a foundation for quantifying river water quality at the catchment scale.

How to cite: Dwivedi, D., Özgen Xian, I., Arora, B., Faybishenko, B., Newcomer, M., Fox, P., Steefel, C., Williams, K., Nico, P., Hubbard, S., and Brodie, E.: A Scale-Adaptive Framework for Modeling Critical Zone Processes and River Water Quality in the East River Watershed, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13922, https://doi.org/10.5194/egusphere-egu25-13922, 2025.

EGU25-14421 | Posters on site | HS8.2.8

Groundwater dynamics in a steep Himalayan catchment: the role of a widespread weathering layer in water storage and transfer 

Kapiolani Teagai, John-Joseph Armitage, Niels Hovius, Léo Agélas, Nobuaki Fuji, Luc Illien, Basanta Raj Adhikari, and Christoff Andermann

The Himalayan region is crucial for providing water resources to millions of people in downstream regions across Asia. However, the processes governing groundwater storage and flow in steep mountain catchments remain poorly understood, particularly regarding the interplay between monsoonal rainfall, infiltration, and groundwater recharge in these highly dynamic landscapes. This study investigates the Kahule Khola watershed in central Nepal, combining field-based approaches encompassing Electrical Resistivity Tomography (ERT), infiltration measurements, and hydrogeochemical analyses, to investigate the pathways and storage mechanisms of groundwater across pre-, during, and post-monsoon seasons. Our findings highlight the critical role of a laterally extensive weathering layer, 10–25 m thick, in regulating hydrological processes. The weathering layer exhibits high infiltration capacities (<24.1 cm/h) that exceed even intense monsoonal rainfall rates (<162.8 cm/h), allowing surface water to rapidly penetrate the subsurface and replenish groundwater stores. The 2D ERT profiles reveal seasonal variations in the saturation of this layer, with significant vertical and lateral flow dynamics linking it to deeper fractured bedrock aquifers. Hydrogeochemical analyses of spring water further demonstrate a bi-compartmentalized flow regimes, where fast and shallow pathways dominate during the monsoon, while slower and long-term storage within the fractured bedrock sustains perennial spring discharge and stream baseflow throughout the dry season. This study enhances our understanding of the hydrological functioning of steep mountain landscapes, emphasizing the dual role of the weathering layer as both a temporary water reservoir and a conduit for deeper aquifer recharge, demonstrating heightened efficiency during monsoon season. By proposing a conceptual model of water transfer and storage in Himalayan catchments, this research provides critical insights into groundwater processes that are fundamental for sustainable water resource management under increasing pressures from climate variability and tectonic activity.

How to cite: Teagai, K., Armitage, J.-J., Hovius, N., Agélas, L., Fuji, N., Illien, L., Adhikari, B. R., and Andermann, C.: Groundwater dynamics in a steep Himalayan catchment: the role of a widespread weathering layer in water storage and transfer, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14421, https://doi.org/10.5194/egusphere-egu25-14421, 2025.

EGU25-14670 | Orals | HS8.2.8

Extreme Winter Precipitation Drives Recharge of Deep Mountain Groundwater 

W. Payton Gardner, Matthew Swarr, Donald Argus, Hilary Martens, Zachary Young, and Zachary Hoylman

Extreme winter precipitation events, associated with frequent and intense atmospheric rivers, deposit significant quantities of water in mountain regions over short periods of time. Precipitation is forecast to become more variable as climate change intensifies; however, it is unclear how that will affect mountain aquifer recharge. Here we use high-precision Global Navigation Satellite Systems (GNSS) surface displacements and elastic deformation models to surface loading to estimate total water storage changes.  Using independent estimates of water stored within shallow subsurface and surface reservoirs, we isolate changes in mountain groundwater storage in two important mountain regions of the western US at high spatial (~30km) and temporal (~ 1 week) resolution. We find that groundwater storage is the dominant component of long-term total water loss within the Sierra Nevada and Cascades, composing up to 95% of the total water lost over the past two decades. However, extremely wet winters, such as that of 2023, can recharge groundwater storage by more than twice the average annual amount, driving the state of groundwater storage from historical lows to above or near-normal conditions over relatively short periods. Further, we find gains in groundwater storage associated with these events are relatively durable, persisting over several proceeding years following the extreme recharge event. Mountain aquifers have been increasingly recognized as a dynamic and critical source of water storage and release to adjacent low-elevation communities; however, persistent declines in mountain aquifer storage have been observed across the western US over the past two decades. In a future with increasingly variable precipitation, the strong influence of extreme events may act to maintain mountain groundwater, sustaining ecosystem health and buffering adjacent areas against drought conditions in between events.

How to cite: Gardner, W. P., Swarr, M., Argus, D., Martens, H., Young, Z., and Hoylman, Z.: Extreme Winter Precipitation Drives Recharge of Deep Mountain Groundwater, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14670, https://doi.org/10.5194/egusphere-egu25-14670, 2025.

EGU25-15141 | ECS | Orals | HS8.2.8

Down Under(ground) – Introducing the Australian Critical Zone Observatory Network 

Simone Gelsinari, Konrad Miotliński, Matthias Leopold, Jessie Weller, and Sally Thompson

The growing global network of Critical Zone Observatories provides exciting insights into how terrestrial and subsurface environments are interconnected, emphasising the value of understanding the Critical Zone as a vertically integrated system.  Yet this network is situated overwhelmingly in the frequently young and post-glacial or glacially-influenced landscapes of the Northern Hemisphere.  The Southern Hemisphere offers diverse landscapes with geologic parent materials spanning the Archaean to the Cenozoic, which have experienced little glaciation relative to the Northern Hemisphere.  The Australian Critical Zone Observatory Network was established in 2020 to provide insights into the structure and functioning of such landscapes on the ancient, chemically depleted, dry and diverse Australian continent. Five sites have been established with a common suite of instrumentation and operating principles, and are working collaboratively to develop Critical Zone datasets in landscapes ranging from rainforest to eucalyptus woodlands, dryland mallee, tropical savannah and rain-dependent agricultural lands.

This talk will introduce the OzCZO – the Australian Critical Zone Observatory Network, the five sites, their instrumentation and opportunities for scientific research within and by making comparisons among the sites.  It will then share some of the initial observations being collected at one of the observatories – the ancient lateritic landscape of the Avon Critical Zone Observatory.  We will illustrate how CZ structure, illuminated by bore logs and geophysics, organises soil physical and chemical properties across the landscape, and reveal how these properties then feed into land management decisions, hydrological functioning, and large-scale ecological health.  The Avon CZO is located within a biodiversity hotspot in the South-West of Australia, where the health of land and waters, and the ecosystems and agricultural production that depend on them, is threatened by both dryland salinity and a drying climate – with outcomes all mediated by the Critical Zone.

All data from OzCZO will be publicly available for use, and the sites are intended to act as an open platform where researchers can develop and test their ideas.  Given the scope for valuable cooperation and comparisons across these sites, we invite researchers at EGU to engage with OzCZO and keep progressing towards a global Critical Zone science.

How to cite: Gelsinari, S., Miotliński, K., Leopold, M., Weller, J., and Thompson, S.: Down Under(ground) – Introducing the Australian Critical Zone Observatory Network, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15141, https://doi.org/10.5194/egusphere-egu25-15141, 2025.

EGU25-17724 | ECS | Posters on site | HS8.2.8

Understanding surface - groundwater interactions in central European upland catchments: the Ahr valley, Germany 

Benoit Abadie, Laura Fracica, Christoff Andermann, Niels Hovius, Michael Dietze, and John Armitage

With a changing climate, major flood events are an increasing risk in many parts of the world, including temperate zones in Western Europe. Recent examples of destructive flooding in central European upland catchments, such as the 2021 Eifel floods in western Germany, highlight the importance of improving our understanding of the mechanisms behind stream response and sediment transport to precipitation events in upland catchments in temperate Western-Europe. The HIdden water and LANDscape ERosion (HILANDER) project that started in spring 2024 has two major goals: 1. To put in place an observatory in the Ahr catchment to characterize how water travels through the critical zone. 2. To incorporate surface/groundwater interactions in models of landscape evolution and river erosion.

The Ahr valley, ranging from 50m to 737m of elevation, is characterized by gently sloped hilltops and a steep, incised river valley. Preliminary recession analyses of the Ahr catchment, performed on data from four existing hydrographs, show a faster flowing aquifer in the upper parts of the catchment and a slow flowing aquifer in the lower regions. This implies that the upper parts of the catchment may be dominated by sub-surface flow through a more permeable shallow layer whereas the streamflow in lower reaches of the catchment is dominated by the deeper underlying aquifer. Two sub-catchments of the upper Ahr river, the Michelsbach, mainly forested and the Huhnenbach, largely agricultural with engineered drainage systems were chosen as study sites. The catchments are instrumented with pressure sensors, turbidimeters and seismometers, to continuously measure streamflow, suspended sediment concentrations, bedload transport and groundwater saturation. Furthermore, springs have been mapped and sampled for stable isotopes, dating and major elements.

Springs are found at both high and low elevations within both sub-catchments, and the locations of these springs do not vary from summer to winter. Observations from the summer spring mapping campaign of June 2024 found that the age of spring-water at high elevation is a mix of young water (ages of 2 to 3 years) and old water (age of 16 years). The presence of both young and old components in the spring water implies multiple pathways for groundwater within the catchment. In January 2025 we found that the ridge tops were saturated with substantial ponding of surface water. Down slope there was either diffuse release of this water or point release at the same locations of springs that were mapped and sampled in the summer. This, along with higher winter oxygen saturation in the springs, points to the potential for interflow during high rainfall events, where water flows laterally through the shallow soil and rock moisture layers (weathering zone) mixing with the groundwater supply. The future continuous monitoring in this critical zone observatory will give insight to the interplay between lateral water pathways in the weathering zone, and deep groundwater reservoirs allowing for a better understanding of how water flow through the catchments can impact erosion and landscape evolution.

How to cite: Abadie, B., Fracica, L., Andermann, C., Hovius, N., Dietze, M., and Armitage, J.: Understanding surface - groundwater interactions in central European upland catchments: the Ahr valley, Germany, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17724, https://doi.org/10.5194/egusphere-egu25-17724, 2025.

EGU25-18247 | Posters on site | HS8.2.8

The International Soil Moisture Network (ISMN): A global hub for in situ observations serving earth system science 

Matthias Zink, Tunde Olarinoye, Fay Boehmer, Kasjen Kramer, Stephan Dietrich, and Wolfgang Korres

Soil moisture is a critical component of the Earth’s hydrological cycle, influencing weather, climate, agriculture, and ecosystems. In situ soil moisture measurements are indispensable for validating satellite observations, calibrating hydrological and land surface models, and advancing our understanding of regional and global water cycles. Unlike remote sensing, in situ measurements provide direct observations of soil moisture variability across temporal and spatial scales, offering a benchmark for numerous environmental applications.

The International Soil Moisture Network (ISMN) serves as a vital repository of harmonized in situ soil moisture data collected from diverse networks worldwide. Since its inception, the ISMN has integrated measurements from over 80 networks with more than 3000 stations at various depths, standardizing and curating them to ensure accessibility and comparability. Beyond offering comprehensive in situ soil moisture data, ISMN disseminates additional environmental variables, including soil temperature, snow depth, snow water equivalent, precipitation, air temperature, surface temperature and soil water potential if they are available from our data providers. ISMN’s quality control framework addresses inconsistencies and errors, enabling researchers and practitioners to confidently utilize its datasets for applications ranging from hydrological modeling to climate change studies. ISMN’s free data access (https://ismn.earth) has fostered global collaboration and supported hundreds of studies in Earth system science.

Ongoing efforts are concentrated on expanding the database by incorporating additional stations and networks from institutional or governmental sources. Further resources are directed towards fortifying the operational system and improve usability to better serve our users. ISMN further contributes to the data-to-value chain on international initiatives like WMO, FAO and GCOS. One example is the contribution to WMO’s yearly Global State of the Water Resources report.  To enhance data quality, ISMN is researching AI-based methods for detecting anomalies such as spikes, dips, and plateaus, showing promising initial results.

How to cite: Zink, M., Olarinoye, T., Boehmer, F., Kramer, K., Dietrich, S., and Korres, W.: The International Soil Moisture Network (ISMN): A global hub for in situ observations serving earth system science, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18247, https://doi.org/10.5194/egusphere-egu25-18247, 2025.

EGU25-18699 | ECS | Orals | HS8.2.8

Elaboration of a geological and hydraulic mapping project of infiltrability potential on the Aix-Marseille Provence Metropole (SE, France) 

Lilas Ruttyn, François Fournier, Philippe Leonide, Borgomano Jean, Bruno Arfib, Sophie Viseur, Laurent Goulet, Olivier Vignoulle, and Narimane Zaabar

The Aix Marseille Provence metropolitan area experiences rapid urbanization that reinforces the need for infrastructure and implies considerable sealing of the substratum This region is a typical arid and Mediterranean environment where rain precipitation can be exceptionally catastrophic. This two factors creates runoff, overflow and flooding in the urban area. One solution to manage the flooding and overflow is to allow more water to penetrate into the soil, by removing the impermeable and anthropic materials where the geological substratum is naturally able to infiltrate the water.

Usually, standard parameters such as: topography, drainage density and hydrological balances, are used to estimate runoff and indirectly find the infiltrability values and ultimately tackle infiltration problematics. These approaches are informatic and mathematics-based that work in a small, delimited and homogeneous area. To integrate this problematics to large scale and heterogenous systems, reservoir geology concepts such as geomorphology, uncertainties of scale change processes or structural geology can be addressed. Therefore, this project aims to understand the geological processes that controls the infiltration potential in the geological substratum and its spatial distribution for the purpose of creating an infiltrability map of the Aix Marseille metropolis.

The goal of this study is to develop a method for predicting the infiltration capacity on a large scale and heterogenous area including urban zone. This involves acquiring local observational data points which classify rock outcrops in 4 “hydraulic types” (HT) defined as follows: HT-1 represents impermeable rocks or soils, where no infiltration is possible; HT-2 represents thin soils with variable porosity and permeability; HT-3 describes rocks with low to very high matrix porosity influenced by clay matrix presence and variable permeability; HT-4 describes rocks with fractures and/or karst networks with low to very high permeability depending on fracture/cavity density, with variable porosity. With the geolocated data points, a map is created on QGIS (a Geographic Information System free software) in order to up-scale the hydraulic types over a larger scale grid by spatial interpolation.

For an even acquisition area, geological heterogeneity and accessibility of outcrops determines the data number needed to upscale hydraulic types. This approach is well-known in reservoir geology and this large-scale project is the opportunity to apply the methodology to  hydrogeology field.

Additionally, to address the lack of visibility of outcrops, subsurface data (shallow well data from the BRGM, Bureau of Geological and Mining Research) will be combined with field observations. Furthermore, a calibration of this method will be required to quantify and to establish thresholds within the Hydraulic Types classification. This project will ultimately provide specific values for infiltration capacity and facilitate flood risk management without having to use complex and costly technologies.

 

Keywords : SIG mapping, infiltration, runoff, geological substratum, stratigraphy, structural geology, heterogeneity, precipitation, de-sealing, available water

 

How to cite: Ruttyn, L., Fournier, F., Leonide, P., Jean, B., Arfib, B., Viseur, S., Goulet, L., Vignoulle, O., and Zaabar, N.: Elaboration of a geological and hydraulic mapping project of infiltrability potential on the Aix-Marseille Provence Metropole (SE, France), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18699, https://doi.org/10.5194/egusphere-egu25-18699, 2025.

EGU25-20210 | Posters on site | HS8.2.8

Integrating Data into the Hydrogeophysical Model: A Case Study of the Orgeval Critical Zone Observatory 

Agnès Rivière, Ludovic Bodet, Maxime Gautier, Alexandrine Gesret, Roland Martin, Sylvain Pasquet, Nicolas Radic, Jose Cunha Teixeira, Marine Dangeard, and Didier Renard

Quantifying the water and heat fluxes at the interface between surface water (SW) and groundwater (GW) is a key issue for hydrogeologists to consider for safe yield and good water quality. However, such quantification with field measurements is not straightforward because the SW-GW changes depend on the boundary conditions and the spatial description of the hydrofacies, which aren't well known and are usually guessed by calibrating models using standard data like hydraulic heads and river discharge. We provide a methodology to build stronger constraints to the numerical simulation and the hydrodynamic and thermal parameter calibration, both in space and time, by using a multi-method approach. Our method, applied to the Orgeval Critical Zone Observatory (France), estimates both water flow and heat fluxes through the SW-GW interface using long-term hydrological data, time-lapse seismic data, and modeling tools. We show how a thorough interpretation of high-resolution geophysical images, combined with geotechnical data, provides a detailed distribution of hydrofacies, valuable prior information about the associated hydrodynamic property distribution. The temporal dynamic of the WT table can be captured with high-resolution time-lapse seismic acquisitions. Each seismic snapshot is then thoroughly inverted to image spatial WT variations. The long-term hydrogeological data (such as hydraulic head and temperature) and this prior geophysical information are then used to set the parameters for the hydrogeological modeling domain. The use of the WT geometry and temperature data improves the estimation of transient stream-aquifer exchanges. Future developments to achieve the fully coupling of the hydrogeophysical model will be presented.

How to cite: Rivière, A., Bodet, L., Gautier, M., Gesret, A., Martin, R., Pasquet, S., Radic, N., Cunha Teixeira, J., Dangeard, M., and Renard, D.: Integrating Data into the Hydrogeophysical Model: A Case Study of the Orgeval Critical Zone Observatory, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20210, https://doi.org/10.5194/egusphere-egu25-20210, 2025.

EGU25-3598 | ECS | Orals | GM2.7

An extended CFD-DEM model based on micropolar fluid for debris flow 

Lian Wang, Xihua Chu, and Hongguang Sun

CFD (computational fluid dynamics)-DEM (discrete element method) model has been widely applied in the simulation of the multiphase flow involving granular materials, but it’s time-consuming for the calculation of a large number of particles with different sizes in DEM. In this study, a model based on the computational micropolar fluid dynamics and discrete element method, viz. a CMFD-DEM model, is proposed to describe the coupling system that consists of gas-liquid two phases and discrete particles with different sizes. In this model, micropolar fluid model is employed to describe the mixture of the pure fluid with fine particles, while discrete element method is used to calculate the motion of the larger particles. In addition, VOF (volume of fluid) method is adopted to track the free surface of the liquid. The implementation of the CMFD-DEM model is based on the open source software, OpenFOAM and LIGGGHTS, and is validated in single particle sedimentation and particles pouring into quiescent water cases. Then, the simulation of debris flow is carried out. The results show that specific dynamic behaviors of debris flow can be reproduced by CMFD-DEM model. The average velocity and runout of debris flow are decreased with the increase of micropolar parameter N/L. Through the comparisons to the exiting results, it suggests that CMFD-DEM model is capable to describe the multi-size effect of the granular materials in debris flow.

How to cite: Wang, L., Chu, X., and Sun, H.: An extended CFD-DEM model based on micropolar fluid for debris flow, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3598, https://doi.org/10.5194/egusphere-egu25-3598, 2025.

Transport of granular materials on Earth and planetary surfaces are at the heart of landscape dynamics and geohazards. These transport phenomena are controlled by particle-scale mechanisms, including particle motion, collisions, and interactions with the ambient fluid, which highlights the importance of particle-resolved measurements in physical experiments. However, despite recent progress in particle tracking velocimetry (PTV) for spherical (and regularly shaped) particles, there still lacks a robust technique in tracking and analyzing the motion of non-spherical particles, particularly because conventional PTV cannot identify moving objects of an arbitrary shape. This limitation largely compromises our particle-scale understanding of the transport of natural granular materials with a wide range of shapes and sizes. To tackle this issue, we propose a novel deep learning-based PTV framework for arbitrarily shaped and sized particles, which consists of a real-time computer vision algorithm called YOLO (you only look once) and an accurate inter-frame matching algorithm based on Kalman filtering. The proposed PTV framework is validated in various granular flow and sediment transport scenarios, using high-resolution data obtained from discrete element method simulations and small-scale physical experiments. Using this new technique, we are able to precisely analyze the kinematics information of spherical, non-spherical, and mixed particles with different concentrations in a series of open channel bedload transport experiments. Scaling relations are obtained between the sediment flux and bed shear stress to reveal the effects of particle shape and composition on the sediment transport dynamics across bedload and sheet flow conditions. The proposed PTV technique and its potential applications are expected to provide a new avenue for future research on the micromechanical aspects of geophysical granular flow and sediment transport.

How to cite: Su, W., Jing, L., and Xu, M.: Deep learning-based particle tracking velocimetry (PTV) for spherical and non-spherical particles: Application to granular flow and sediment transport, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7708, https://doi.org/10.5194/egusphere-egu25-7708, 2025.

Step-pools are common bedforms in mountain streams and have been utilized in river restoration or fish passage projects around the world. Step-pool units exhibit highly non-uniform hydraulic characteristics which have been reported to closely interact with the morphological evolution. Further understanding towards these interactions builds the basis for better prediction of channel evolution and more advanced design of artificial step-pool system. However, detailed information on the flow-morphology interactions has been limited due to the difficulty in measuring the flow structures or the flow forces in a step-pool unit.

To fill in this knowledge gap, we established an approach combining physical experiment and computational fluid dynamics (CFD) simulation for a step-pool unit made of natural grains at six flow conditions. Structure from motion (SfM) was used to capture the detailed 3D reconstructions of the bed surfaces with various conditions of pool scour. The hydraulic measurement was applied both as input data at the inlet boundary and also in the validation for the CFD model. The high-resolution 3D flow structures for the step-pool unit were visualized, as well as the distributions of flow forces from both pressure and shear stress.

The results illustrate the segmentation of flow velocity downstream of the step, i.e., the integral recirculation cell at the water surface, streamwise vortices formed at the step toe, and high-speed flow in between, resulting from the complex morphology of the step-pool unit. Both the recirculation cells at the water surface and the step toe perform as energy dissipaters to the flow with comparable magnitudes. Pool scour development during flow increase leads to the expansion of the recirculation cells until step-pool failure occurs. Significant transverse variability of the flow forces from both the shear stress and pressure has been revealed. The flow forces in both streamwise and transverse directions are closely related to the flow structures and morphology in the unit. The ratios between skin and form drag have large variations at low flows while show a relatively limited range of 0.05-0.1 at high flows, suggesting a small proportion occupied by the skin resistance in the total flow resistance in the step-pool channel. The drag coefficient of the step-pool unit is around 0.3 at high flows. Our results highlight the feasibility of the approach combining physical and numerical modeling in investigating the complex flow-morphology interactions of step-pool features.

How to cite: Zhang, C., Hassan, M., and Xu, Y.: Investigating interactions between flow and morphology in a step-pool unit combining physical and numerical modeling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7900, https://doi.org/10.5194/egusphere-egu25-7900, 2025.

EGU25-7958 | ECS | Posters on site | GM2.7

Finite-Size Effects in Geophysical Granular Flow from a Nonlocal Rheology Perspective 

Jiacheng Xia, Lu Jing, and Ming Peng

Geophysical granular flow is ubiquitous in nature and plays a crucial role in shaping the landscape (hillslope creep, riverbed evolution) and causing geohazards (landslide, debris flow). Small-scale models are an effective way to understand these natural phenomena at large scales. However, finite-size effects inevitably occur due to the multi-scale nature of granular materials, hindering integration of mechanisms obtained from small-scale investigations and continuum models (e.g., granular flow rheology) for large-scale applications. Here we use granular column collapse as a model case to address finite-size effects in granular flows from a novel rheological perspective. We computationally simulate column collapse of varying system-to-particle size ratios using the discrete element method and extract detailed local rheological information during the flow via a coarse-graining technique. We find a disproportional increase in the dimensionless runout distance with the system-to-grain size ratio and a significant difference in the dynamic process. This discrepancy is reflected in the μ(I) curve as non-collapsed data at low inertial number regimes, but casting the data into a non-local rheology framework proposed by Kim and Kamrin (2020) leads to data collapse onto a single master curve for all simulations. This indicates that the finite-size effect is controlled by velocity fluctuations at the grain scale and is a manifestation of the non-locality of granular materials. As a result, the introduction of an intermediate length scale that reflects velocity fluctuations is expected to enable accurate modeling of geophysical granular flows with varying system and particle sizes in a unified continuum framework. It also provides a new perspective for continuum modeling of polydispersity, size segregation, hysteresis, and other size-dependent phenomena in geophysical granular systems.

How to cite: Xia, J., Jing, L., and Peng, M.: Finite-Size Effects in Geophysical Granular Flow from a Nonlocal Rheology Perspective, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7958, https://doi.org/10.5194/egusphere-egu25-7958, 2025.

EGU25-8700 | Posters on site | GM2.7

Quantification of intense transport of fractions of stratified bimodal bed load based on measured distributions of velocity and concentration 

Vaclav Matousek, Jan Krupicka, Tomas Picek, and Lukas Svoboda

We present the results of laboratory experiments investigating the intense transport of bimodal bed load under high bed shear conditions in a tilting flume. Particles of two lightweight sediment fractions, differing in size, tend to separate during transport above the plane surface of an eroded mobile bed. Coarser fraction particles are predominantly present in the collisional layer above the bed, while finer fraction particles are primarily concentrated in the interfacial layer, which develops between the eroded bed and the collisional layer. This observed stratification of transported fractions influences their respective contributions to the total bed load discharge through the flume. Vertical distributions of local velocity and volumetric concentration were measured across the flow depth for each fraction separately, allowing the determination of each fraction's proportion in the total discharge. The experimental results were combined with a previously collected dataset to compare the discharges of bimodal and unimodal sediments under hydraulically similar conditions. Additionally, the experimentally determined discharges were evaluated against predictions from transport models designed for intense unimodal and bimodal bed loads.

How to cite: Matousek, V., Krupicka, J., Picek, T., and Svoboda, L.: Quantification of intense transport of fractions of stratified bimodal bed load based on measured distributions of velocity and concentration, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8700, https://doi.org/10.5194/egusphere-egu25-8700, 2025.

EGU25-8745 | ECS | Posters on site | GM2.7

Reliability-Based Analysis of Initiation of Sediment Motion on Movable Bed 

Selman Baysal, V. Ş. Özgür Kırca, and Manousos Valyrakis

Sediment transport dynamics are of great importance in understanding geophysical flows, where determining the threshold conditions for the initiation of sediment motion presents a complex challenge. In a pioneering work, Shields (1936) established the Shields’ criterion to assess the critical shear stress (τc) required for sediment motion in non-turbulent flows. Although this approach has significant advantages, including a robust empirical foundation and the implementation of non-dimensional critical shear stress, it is valid for limited conditions since it oversimplifies vital aspects such as sediment heterogeneity and complex flow interactions.

In turbulent flows, the effective critical shear stress acting on a grain may become higher than that measured in the case of laminar flows (i.e., the average critical stress, τc, defined by Shields, 1936) as a result of fluctuations in the shear stress (τ′). Owing to this, in geophysical turbulent flows near the threshold of motion, neither the driving nor the resisting parameters of sediment motion have crisp values; instead, they may be considered probabilistic parameters. The reliability-based approach is applied here in to handle the complex nature of the initiation of sediment motion.

This study aims to present preliminary results of research that aims to enhance the knowledge of incipient motion by applying a reliability-based analysis of Shields’ criterion based on the theory and empirical equations adopted by Zanke (2003). In this analysis, the turbulence parameter (n) and angle of repose (ϕ) are introduced as key parameters regarding the initiation of sediment motion. These parameters are generated as random variables by means of Monte Carlo Simulations, introducing various probabilistic distributions (e.g., normal, log-normal, triangular, gamma) and statistical moments (e.g., mean, standard deviation).

By simulating a wide range of angles of repose and turbulence parameters with Monte Carlo Simulations, the inherent uncertainties in sediment transport and the complexity of hydrodynamic models are incorporated. In this work critical shear stresses of thousands of grains are assessed for different grain Reynolds numbers. As a result, threshold of motion curves are probabilistically derived, indicating confidence for grain entrainment, and establishing a model that enables risk assessment and decision-making for a wide range of scenarios. Comparisons of model results with empirical data show that the model captures the complex physical process.

How to cite: Baysal, S., Kırca, V. Ş. Ö., and Valyrakis, M.: Reliability-Based Analysis of Initiation of Sediment Motion on Movable Bed, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8745, https://doi.org/10.5194/egusphere-egu25-8745, 2025.

Avalanches of dry granular materials, such as rocks, snow, and ice, are chief contributors to hazardous geophysical flows in nature. A key problem hampering progress in predicting the destructiveness of such hazards is the poorly understood dependence of the flow velocity on the physical properties of the grains constituting a given material. In particular, their usually irregular, non-spherical shapes prevent application of rigorous theories, which were derived for spherical grains. In addition, we do not have a good empirical grasp of the issue, as evidenced by the failure of existing scaling laws across flows of different granular materials when applied to measurements and numerical simulations for idealized flow geometries. Here, we report a scaling law for the steady-state velocity of homogeneous granular flows down rough inclines. It holds for granular materials consisting of irregularly-shaped but relatively uniformly-sized grains descending rough slopes. Laboratory chute experiments and numerical simulations for a diverse range of granular materials corroborate its validity and generality. It exhibits a power-4/3 dependence on the flow thickness, as opposed to the power-3/2 dependence suggested by previous scaling laws. It is also unique in the aspect that it depends only on a single parameter characterizing the granular material: the dynamic angle of repose. This suggests that, quite surprisingly, most of the physical complexity associated with the composition and shape of a material's grains boils down to its bulk ability to resist externally-driven shearing.

How to cite: Pähtz, T.: General scaling law for the velocity of steady, homogeneous granular flows down rough inclines, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9678, https://doi.org/10.5194/egusphere-egu25-9678, 2025.

EGU25-9842 | ECS | Orals | GM2.7

Turbulence increases sediment transport 

Daniel Rebai, Katinka Koll, Alessio Radice, Jochen Aberle, and Francesco Ballio

In steady, fully developed flows over erodible beds, the average bed shear stress is generally the dominant factor governing sediment flowrate. However, fluctuations induced by turbulence can play a significant role in altering sediment transport dynamics. This study investigates the effects of such turbulence by conducting flume experiments with flow disturbances created by various cylinder arrays placed in the flow. To measure the turbulent flow field, Laser Doppler Velocimetry (LDV) was employed, while bed shear stress was quantified using a shear plate. The bedload motion was analysed using Particle Tracking Velocimetry (PTV), which allowed for the quantification of key variables such as sediment concentration, velocity, and sediment flowrate. A descriptive model was developed to capture the relationship between these primary variables and both the average and fluctuating components of the flow. Our results show that with increasing turbulent fluctuations, both sediment concentration and velocity rise at a fixed mean shear stress. Notably, turbulence influences concentration more strongly than velocity.

How to cite: Rebai, D., Koll, K., Radice, A., Aberle, J., and Ballio, F.: Turbulence increases sediment transport, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9842, https://doi.org/10.5194/egusphere-egu25-9842, 2025.

EGU25-10237 | Orals | GM2.7

Unified flow rule of undeveloped and fully-developed dense granular flows down rough inclines 

Yanbin Wu, Thomas Pähtz, Zixiao Guo, Lu Jing, Zhiguo He, and Jinchuan Zhang

We report on chute measurements of the free-surface velocity $v$ in dense flows of spheres and diverse sands and spheres-sand mixtures down rough inclines. These and previous measurements are inconsistent with standard flow rules, in which the Froude number $v/\sqrt{gh}$ scales linearly with $h/h_s$ or $(\tan\theta/\mu_r)^2h/h_s$, where $\mu_r$ is the dynamic friction coefficient, $h$ the flow thickness, and $h_s(\theta)$ its smallest value that permits a steady, uniform dense flow state at a given inclination angle $\theta$. This is because the characteristic length $L$ a flow needs to fully develop can exceed the chute or travel length $l$ and because neither rule is universal for fully-developed flows across granular materials. We use a dimensional analysis motivated by a recent unification of sediment transport to derive a flow rule that solves both problems in accordance with our and previous measurements: $v=v_\infty[1-\exp(-l/L)]^{1/2}$, with $v_\infty\propto\mu_r^{3/2}\left[(\tan\theta-\mu_r)h\right]^{4/3}$ and $L\propto\mu_r^3\left[(\tan\theta-\mu_r)h\right]^{5/3}h$.

How to cite: Wu, Y., Pähtz, T., Guo, Z., Jing, L., He, Z., and Zhang, J.: Unified flow rule of undeveloped and fully-developed dense granular flows down rough inclines, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10237, https://doi.org/10.5194/egusphere-egu25-10237, 2025.

Progressive slope steepening can trigger episodic dry sand avalanches, resembling landslides commonly observed in natural environments. Similarly, gradual river incision can induce periodic slope instability and failures. To thoroughly investigate the impact of gradual river incision on catchment topography and slope dynamics, we conduct a series of idealized dry sandbox experiments. This simple setup is expected to provide a deeper understanding of the patterns and dynamics of landslides in mountainous regions.

In the experiments, dry sand is removed by applying negative suction pressure through a nozzle traversing prescribed paths over the topography. This process simulates river channel incision into the sand substrate and triggers avalanches on adjacent slopes. The experimental setup consists of a simple box filled with dry sand, equipped with a suction mechanism inspired by the extrusion nozzles used in 3D printing. Unlike 3D printing, where material is added, negative pressure at the nozzle is used to extract material instead.

To validate the system, we first employ a vertically descending suction nozzle at a controlled rate to produce an expanding conical pit. This simple setup allows us to test the suction mechanism and ensure consistent material removal. Subsequently, we simulate river incision by utilizing an idealized curved path designed to mimic the geometry of an incising river. Initially, the nozzle was manually guided along this path to replicate the incision process. In later experiments, a computer-controlled traversing system is implemented to ensure greater precision and reproducibility.

We then explore imposed motions along the main river channel and incorporate tributaries to explore the river incision processes. The results, including the formation of ridges, avalanches, and slope adjustments, are analyzed and compared with computational predictions derived from an eikonal model. This comparison provides valuable insights into the behavior of slopes under conditions of gradual river incision and elucidates the mechanisms driving slope instability and morphological evolution in natural catchments.

How to cite: Chang, E. and Capart, H.: Experimental Analogue Modeling of Slope Dynamics Induced by Gradual River Incision Using a Controlled Suction Nozzle in Dry Sandbox Experiments, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12716, https://doi.org/10.5194/egusphere-egu25-12716, 2025.

EGU25-13548 | Posters on site | GM2.7

Shallow-water continuum modelling of dry granular flows in partailly obstructed chutes  

Rui Miguel Ferreira and Solange Mendes

We employ data about a dry granular flow down a 19º smooth-walled chute, partially obstructed at the downstream end, to verify the solution of a shallow-water continuum model. The system of conservation equations is based on depth-averaging the ensemble-averaged mass, momentum and fluctuating kinetic energy equations:

(1)  $\partial_t \left(\phi h \right) + \partial_x \left(\phi h u \right) = - \partial_t z_b$

(2)  $\partial_t \left( \rho h u \right) + \partial_{x} \left( \rho h u^2 \right)  = -\partial_{x} \left( \rho g h^2 / 2 \right) - g \rho h \, \partial_{x} z_b  - \tau_b$

(3) $\partial_{t} z_b = - \left( E(x,t) - D(x,t) \right)$

(4) $P = f(\phi) f(e,k,\phi_c) \rho_g T$

(5) $-Q^\prime + \frac{1}{2}\tau_b u/h - \Gamma = 0$

where $x$ is the distance, $t$ is time, the conservative variables are the elevation of the granular bed, $z_b$, the equivalent depth of flowing granular material $\phi h$ and flow momentum $\rho \phi h$, where $\phi$ is the solid fraction, $h$ the granular depth and $u$ the depth-averaged longitudinal velocity, $\tau_b$ is the wall stress, $E$ and $D$ are the rates of particle pick-up and deposition, respectively, $e$ is the normal coefficient of restitution, $k$ is particle stiffness, $\phi_c$ is the critical solid fraction, $\rho_g$ is the density of the solid particles, $\rho = \rho_g \phi$, $\Gamma$ is the rate of dissipation of fluctuating kinetic energy and $Q^\prime$ is the flux of fluctuating kinetic energy at the bottom wall.  The solid fraction is determined from (4) as a function of the granular pressure $P$ (considered hydrostatic) and the granular temperature $T$.

Preliminary results of simulations with borosilicate spheres ( g/cm3 and coefficient of restitution ), with  and  as tuning parameters, indicate that the celerity of the jamming wavefront is well-reproduced. The jump strength and the head losses are not in full agreement, requiring adjustments in the equation of state (4).

 

Acknowledgements

Portuguese Foundation for Science and Technology (FCT) through the PhD scholarship PD/BD/150693/2020, project PTDC/ECI- EGC/7739/2020 and CERIS funding UIDB/04625/2020.

How to cite: Ferreira, R. M. and Mendes, S.: Shallow-water continuum modelling of dry granular flows in partailly obstructed chutes , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13548, https://doi.org/10.5194/egusphere-egu25-13548, 2025.

EGU25-13625 | Orals | GM2.7

Formation and evolution of sediment ribbons in open-channel flow 

Olivier Eiff and Michele Trevisson

The formation and evolution of sediment ribons over a uniform sediment bed in an open-channel flow was investigated via a stereo-photogrammetric system to measure the bed evolution in combination with a stereo-PIV system to measure the three-component velocity field in a cross-sectional plane above the bed. The formation of ribbons is observed to be triggered by the initially meandering low and high-speed streaks sharing the same spanwise wavelength as the fully-developed ribbons.  When the ribbons are fully developed, the streaks are locked in place with low-speed streaks over the ridges and high-speed streaks over the troughs with strong secondary flows.  The lateral stabilization appears to be facilitated by the stable  streaks near the wall.

How to cite: Eiff, O. and Trevisson, M.: Formation and evolution of sediment ribbons in open-channel flow, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13625, https://doi.org/10.5194/egusphere-egu25-13625, 2025.

EGU25-14061 | ECS | Posters on site | GM2.7

Experimental investigation on the formation and failure of landslide dam using inertial navigation method 

Ran Li, Yi-ming Li, Tong-Tong Mu, and Hong-yang Dai

Landslides in narrow valleys may block adjacent rivers and dam the incoming water flow. The collapse of these landslide dams may lead to catastrophic flooding downstream. The measurement and early warning of dam failures is an important issue in geomorphic processes. However, Optical and radar-based monitoring methods are not suitable for deep internal probing of a dam, which is necessary for dynamic measurement and early warning. In this study, the acceleration of a smart rock in the simulation dam was measured using inertial navigation method. It is found the acceleration response of smart rocks is detected more than 20 seconds before external observations of dam failure. Buried at different positions within a dam, smart rocks exhibit distinct temporal and data form responses to dam failure. Smart rocks located deeper within the dam show multiple acceleration fluctuations before the actual failure occurs. We hope that the measurement data provided by smart rocks will assist in developing multi-scale models of dam failure.

How to cite: Li, R., Li, Y., Mu, T.-T., and Dai, H.: Experimental investigation on the formation and failure of landslide dam using inertial navigation method, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14061, https://doi.org/10.5194/egusphere-egu25-14061, 2025.

EGU25-14133 | Orals | GM2.7

Energetic kinetic of debris flow in a horizontal chute using centroid vector displacement method 

Hui Yang, Zhipeng Chi, Quan Chen, and Yue Xu

Debris flows, as a type of large-scale geological disaster, are a global focus regarding their formation boundary, kinematic properties and deposit morphology. In small-scale laboratory simulations, factors such as water content, equivalent grain size, grain size ratio and aspect ratio significantly influence the formation boundaries and flow regime. Quantifying the effects of these numerous variables is a crucial prerequisite for advancing research on geological disasters represented by debris flows. We conducted simulations of the debris flow triggering process within a horizontal chute and used the proposed centroid vector displacement method to quantitatively assess the kinetic characteristics from an energetic perspective. By integrating the influence of water content into the traditional Bond number, we were able to clearly differentiate three distinct collapse regimes. Through modulation of the size and density ratios, we explored the distribution of intensity for various mechanisms along the flow direction. To characterize the relative strength of diffusion and buoyancy effects on the length scale, we introduced a dimensionless parameter λ. This parameter enabled us to define the boundary conditions necessary for the formation of core-band patterns.

How to cite: Yang, H., Chi, Z., Chen, Q., and Xu, Y.: Energetic kinetic of debris flow in a horizontal chute using centroid vector displacement method, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14133, https://doi.org/10.5194/egusphere-egu25-14133, 2025.

Alluvial fans develop at the base of mountain fronts, where rivers emerge from the constrained mountain area onto the plain. Acting as a transition zone between mountain streams and alluvial rivers, the fan-river system is typically characterized by a slope break in the bed profile, a significant discontinuity in bed surface sediment fining from gravel-sized to sand-sized, and a sudden increase in channel width. In large rivers with great morphological diversity and strong human interference, the shift between upstream and downstream river morphology and sediment dynamics within the alluvial fan-river system exhibits a more complex process. However, this phenomenon remains insufficiently documented and lacks comprehensive analysis.

Here, we take the middle Yangtze alluvial fan as an example and use field observations and numerical modeling to improve the understanding of the large-scale alluvial fan-river system. The result shows that, in contrast to other alluvial fan-river systems, the Yangtze alluvial fan downstream of the Three Gorges Valley had no obvious breaks in the recent bed profile. In addition, the channel width showed an abrupt increase at Zhicheng, followed by a narrowing trend beginning at Chenjiawan. After the Three Gorges Dam (TGD) operation in 2003, the erosive water released from the TGD induced significant erosion, however, the spatial pattern of the bankful width remained stable. The bed profile exhibited increasing variability but continued to lack a distinct slope break; The transition in surface material from gravel to sand was observed throughout approximately 60 kilometers and the location migrated 40 kilometers downstream in the post-TGD period, with gravel and sand patches alternating randomly; Zhicheng and Chenjiawan are two characteristic locations marking the shifts in the mode of sediment transport in the middle Yangtze alluvial fan-river system. For sand transport mode, the reach upstream of Zhicheng had sand transported in suspension, whereas the downstream reaches were dominated by mixed-load transport. For gravel transport mode, gravel from upstream, mostly in the 25–50 mm grain size range, was selectively transported downstream of Zhicheng and deposited at Chenjiawan; The sediment dynamics in the Yangtze alluvial fan-river system were controlled by the width variability and distributary streams. The deposition of fine sand upstream of the gravel smoothed the previously deposited gravel fan profile, resulting in the absence of a slope break in the bed profile. Since 2003, the pattern of the sediment transport mode remained stable despite some local adjustments. This stability is attributed to the stable fan-river morphology induced by the strong resistance of riverbank lithologies and the Jingjiang Great Levee constraints.

How to cite: He, Z., Sun, Z., Li, Y., Luan, H., and Qu, G.: Large-scale alluvial fan-river system of the middle Yangtze River: morphological diversity, grain size discontinuity, and sediment dynamics complexity, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14540, https://doi.org/10.5194/egusphere-egu25-14540, 2025.

EGU25-14717 | Posters on site | GM2.7

Modeling Debris Flow Transitions: Experimental Validation and Field-Scale Application 

Chieh-Ya Liao, Yi-Ling Tsai, and Chi-Yao Hung

Debris flows, prevalent in mountainous regions, exhibit distinct dynamics depending on whether they occur over bedrock (rigid bed) or accumulated deposition (erodible bed). Understanding the transition between these bed types is essential for hazard prediction and mitigation. This study improves an existing unsteady, non-uniform debris flow model to more accurately simulate the evolution of flow depth and velocity under varying boundary conditions. The improved model is grounded in mass, momentum, and kinetic energy conservation principles, incorporating a linearized μ(I) rheology to describe granular flow behavior and Coulomb friction along sidewalls, ensuring a realistic representation of debris flow mechanics.

To validate the improved model, granular dam break experiments were conducted in a narrow glass channel (3.5 m long, 0.04 m wide) with varying downstream deposit depths to establish different basal boundary conditions. High-speed camera footage and Particle Tracking Velocimetry (PTV) were employed to capture granular motion and generate velocity fields. The model exhibited good agreement with experimental results, accurately predicting the flow depth and velocity evolution during the transition between rigid and erodible beds.

Furthermore, the model was applied to field-scale debris flows at the PuTunPunas River in southern Taiwan, a site that has experienced several debris flow events over the past decades. Channel width variations at this site were incorporated into the model to assess erosion potential and flow behavior under real-world conditions. Comparisons with field observations confirmed the model’s capability to simulate debris flow transitions and erosion processes in natural channels, offering valuable insights for hazard assessment and mitigation in mountainous regions.

How to cite: Liao, C.-Y., Tsai, Y.-L., and Hung, C.-Y.: Modeling Debris Flow Transitions: Experimental Validation and Field-Scale Application, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14717, https://doi.org/10.5194/egusphere-egu25-14717, 2025.

EGU25-14812 | ECS | Orals | GM2.7

Slowflows: Experiments and numerical simulations 

Parameshwari Kattel, Chet N. Tiwari, and Shiva P. Pudasaini

Due to various destabilizing factors such as hydro-thermo-mechanical degradation, and earthquakes, the strength of the Earthsurface material may decrease, leading to increased slow earthflow events. Earthflows often cause extensive damage to infrastructure and permanently change the landscape pattern. However, the earthflows have received much less attention compared to their fast-moving counterparts, like avalanches, landslides, and debris flows. Here, we present some novel laboratory experiments simulating slowflows to understand their initiation, movement, and long-term morphological evolution by using a highly viscous material, the molten jaggery, locally found in Kathmandu. The tremendously slowly deforming and moving jaggery is assumed to represent earthflows. Experimental results demonstrate some key aspects of slowflow dynamics of earth materials and seminally contribute to the systematic understanding of earthflow processes. We simulate the slowflow propagation process by using a dynamic earthflow model. Simulation results capture some essential features of the massively viscous, exceptionally slowly deforming, and moving earth surface materials. 

How to cite: Kattel, P., Tiwari, C. N., and Pudasaini, S. P.: Slowflows: Experiments and numerical simulations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14812, https://doi.org/10.5194/egusphere-egu25-14812, 2025.

EGU25-15011 | ECS | Orals | GM2.7

Suspended Sediment Concentration Analysis Using Remote Sensing and Machine Learning Approach 

Srikanth Bhoopathi, Manali Pal, and Harshitha Choubey

This study employs remote sensing technology to thoroughly analyse sediment dynamics in expansive aquatic environments, with a specific focus on the Ganga River basin. The investigation spans from 2007 to 2011, utilizing Medium Resolution Imaging Spectrometer (MODIS) MYD09A1.061 Aqua Surface Reflectance 8-Day Global data to assess Suspended Sediment Concentration . By integrating ground-based silt data with satellite data, the study captures temporal variations in suspended sediment levels. The Google Earth Engine (GEE) platform was employed to process sensor imagery and calculate reflectance data, enabling accurate computations for specific time intervals. To further analyse the data, Support Vector Regression (SVR) model was developed. This model analyse changes in reflectance data  to corresponding  observed silt measurements, providing insights into sediment behavior. The results from this model are presented using 2D graphs, highlighting the  effectiveness of remote sensing technology in understanding the sediment dynamics in large river systems. This research offers significant advancements in  methods for monitoring and maintaining water quality in aquatic environments.

How to cite: Bhoopathi, S., Pal, M., and Choubey, H.: Suspended Sediment Concentration Analysis Using Remote Sensing and Machine Learning Approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15011, https://doi.org/10.5194/egusphere-egu25-15011, 2025.

Sediment transport in turbulent flows is one of the classical topics in rivers and coastal engineering studies. Due to a lack of general description of interphase interactions, the numerical studies are limited by separately describing the motion of sediment particles in the form of bedload or suspended load depending on the relative importance of particle-particle and particle-turbulence interactions. In this paper, a Reynold-averaged Euler-Lagrange model is developed to study bedload and suspended load simultaneously where the interphase interactions are described in a unified mechanical framework. The inter-particle interactions are resolved and the flow turbulence is described by a modified two-phase k-epsilon turbulence model. Particle-fluid interactions at the volume-averaged scale are characterized by the drag force, the pressure gradient force and the lift force. The effects of the interstitial fluid on particle contacts are taken into consideration by formulations of coefficient of restitution and friction coefficient. A modified Continuous Random Walk (CRW) model is adopted to characterize the stochastic motion of the sediment particles. The effectiveness of the model in describing particle-turbulence and particle-particle interactions is firstly demonstrated by comparison with experiments of sediment transport in bedload and suspended load separately. The model is further applied to the study of sediment transport in sheet flows. Contributions of particle-turbulence and particle-particle interactions to the flow structure, the total transport rate and the rheology of particle-fluid mixtures are analyzed.

How to cite: Li, W.: A general description of interphase interactions in Reynolds-averaged Euler-Lagrange simulations of turbulent sediment transport: from bedload to suspended load, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15155, https://doi.org/10.5194/egusphere-egu25-15155, 2025.

Bedload transport, critical in various natural and engineering systems, involves the complex interaction between particles and flowing water. Predicting bedload transport rates has long been a focal point of interest due to its significance in understanding river dynamics. Pioneering contributions from Einstein and Bagnold have led to substantial progress in this field derived from extensive laboratory and in-situ observations, which are yet to achieve the desired accuracy when validated against real-world hydrological data. The discrepancies in predictions can partly be attributed to the difficulties in accurately capturing the movements of near-bed particles and the flow field characteristics.

This paper presents a numerical investigation via Computational Fluid Dynamics-Discrete Element Method into detailed observations on particle movements and flow characteristics of bedload transport. It provides a thorough review of the assumptions and theories prevalent in current bedload models. Simulations have been conducted covering flow velocities ranging from below the generally accepted critical Shields number to the onset of bedform formation. We analyze particle trajectories and statistical behaviors under various conditions, focusing on both the motions of individual particles and the collective evolution of bedforms, and our primary results include: 1. The incipient motion of particles is a gradual process that can occur before reaching the generally accepted critical Shields number. 2. The emergence and development of bedforms under varying conditions. 3. Observations on the relationship between particle movement characteristics and the shear conditions. These findings enhance our understanding of particle-scale dynamics in bedload transport, providing a foundation for evaluating and improving existing models for predicting transport rates.

How to cite: Li, X., Zhao, T., and Xu, B.:  Flow Characteristics and Particle Kinematics in Bedload Transport: a CFD-DEM investigation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15234, https://doi.org/10.5194/egusphere-egu25-15234, 2025.

Assessing particle-scale interactions and transport phenomena is essential yet complex within geophysical flows found in both natural and artificial settings. This research introduces the design, validation, and calibration of a spherical inertial sensor particle meticulously engineered to achieve full kinematic equivalence with a solid sphere. By employing Micro-Electro-Mechanical Systems Inertial Measurement Unit (MEMS-IMU) technology, this low cost 40 mm particle can measure triaxial acceleration up to ±16g and triaxial angular velocity up to ±2000°/s, operating at a high sampling rate of 1000 Hz over a duration of one hour. The sensor particle possesses a dual-layered spherical configuration deliberately crafted to ensure alignment in shape, density, center of mass, moment of inertia, and elastic modulus with that of a solid sphere. Its performance is rigorously assessed, validated, and calibrated through a series of physical experiments. Furthermore, a data enhancement technique grounded in lubrication theory is invented to mitigate technical challenges associated with accelerometer saturation and temporal resolution. This method enables our sensor particle to accurately capture particle collision processes within liquid environment, which proves challenging with conventional approaches. This investigation offers a foundational instrument for large-scale particle motion studies, such as those related to debris flows, facilitating, for the first time, the precise measurement of the dynamic behavior of individual particles within a substantial ensemble.

How to cite: An, Y., Jiao, J., and Zhang, L.: Spherical Inertial Sensor for Measuring Particle-Scale Interactions in Geomorphic Flows with Full Kinematic Equivalence, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15433, https://doi.org/10.5194/egusphere-egu25-15433, 2025.

We have investigated the modeling of collisional bed-load transport with a focus on continuum approaches for granular flow. A frictional-collisional framework, combining the Coulomb model and the kinetic theory of granular flows, is proposed to address the limitations of classical kinetic theory, which fails to accurately reproduce results from coupled fluid–discrete simulations. These discrepancies are attributed to assumptions of negligible interparticle friction and the absence of a saltation model in continuum formulations. 

To guide model development, the fluctuating energy balance obtained from discrete simulations is systematically compared with kinetic theory predictions. The analysis reveals that interparticle friction significantly affects the radial distribution function and increases energy dissipation, aligning with previous findings. Additionally, a saltation regime is identified, causing deviations from the viscosity and pseudo-thermal diffusivity laws of kinetic theory in dilute regimes. 

Building on these insights, the two-fluid model is modified to incorporate interparticle friction and coupled with a saltation model. The results demonstrate that for inelastic, frictional particles, interparticle friction primarily governs energy dissipation, and the macroscopic granular flow behavior is independent of microscopic particle properties. The enhanced model successfully reproduces the 𝜇(𝐼) rheology in the dense regime of granular flow. Experimental validation confirms significant improvements in predicting granular flow behavior, highlighting the model’s effectiveness in capturing key physical processes. 

How to cite: Chauchat, J., Chassagne, R., and Bonamy, C.: A Continuum Framework for Modeling Frictional-Collisional Interactions in Bed-Load Transport: Insights from Discrete Element Simulations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16152, https://doi.org/10.5194/egusphere-egu25-16152, 2025.

EGU25-17293 | ECS | Orals | GM2.7

Dispersion - Erosion Coupling in Landslides 

Jeevan Kafle, Bekha R. Dangol, and Shiva P. Pudasaini

Non-hydrostatic dispersive models can better describe the landslide motion. Following a dispersive wave equation and a mechanical erosion model for mass flows, here, we develop a novel dynamically coupled dispersion-erosion wave model that combines these two very essential complex processes. The newly developed model for landslide recovers the classical dispersive water waves and dispersive wave equation for landslide as special cases. We present several exact analytical solutions for the coupled dispersion-erosion model. These solutions are constructed for the time and spatial evolution of the flow depth. Solutions reveal that the dispersion and erosion are strongly coupled as they synchronously control the landslide dynamics. The results show that the wave dispersive wave amplifies with the increasing particle concentration, decreasing earth pressure, higher gravitational acceleration, increased slope angle and increased basal friction. The important novel understanding is that the intensity of the dispersive wave increases when erosion and dispersion are coupled. The results indicate the essence of proper selection of the initial and boundary conditions while solving applied and engineering problems associated with the dispersive - erosive mass transport. This provides the foundation for our understanding of the complex dispersion and erosion processes and their interplay.

How to cite: Kafle, J., Dangol, B. R., and Pudasaini, S. P.: Dispersion - Erosion Coupling in Landslides, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17293, https://doi.org/10.5194/egusphere-egu25-17293, 2025.

EGU25-18148 | Posters on site | GM2.7

The Fractal and Topological Metrics for Assessing Three-Dimensionality in Dune Morphology  

Sree Sai Prasad Bodapati and Venu Chandra

Dunes are ubiquitous in river, marine, desert and Martian environments. The flow of fluid 
over mobile bed results in evolution of dunes of different sizes and shapes. The shape of dune 
has critical role in sediment transport and interacting with flow. Earlier studies assumed the 
dune shape as a triangle (2-Dimensional) to study the flow field over dunes. However, dunes 
are highly three dimensional and their 3D patterns can increase the form drag compared with 
equivalent 2D dunes in similar flows. Pearson correlation, 2D spatial correlations are used to 
describe three dimensionality of dune in previous studies. A robust methodology to quantify 
3D bed forms and linking it to the flow needs to be developed. In this study, experiments are 
conducted to form 3D dunes on plane bed with non-uniform fine sand (d50 = 0.395 mm, σg = 
1.56) under sub critical flow conditions. The bed morphology is continuously monitored 
using ultrasonic ranging probes (URS) placed 5 cm c/c distance in 1 m wide flume. 
Experiments are performed till equilibrium state is achieved and continued further (2 hrs) to 
observe the bed changes. The equilibrium bed is measured at 2 cm resolution with a laser 
distance meter. The 3D velocity components and suspended sediment concentration are 
continuously measured using down looking Accoustic Doppler Velocimeter (25 Hz). Signal 
processing techniques are used to remove outliers, to smoothen the local fluctuations and 
identification of dune crest and troughs. In addition to 2D correlation and Pearson correlation 
coefficient, Fractal dimensions and topological metrics are also used to asses three 
dimensionality of the sediment bed. Roughness of the sediment bed is quantified using 
standard deviation of bed elevation. From the experiments, it was observed that three 
dimensionality is reduced with an increase in discharge. The spatial data is transformed into 
frequency domain. Periodicity of the process is analyzed from harmonics and spatially 
averaged spectrums. The height and length of dunes is modelled using exponential fits and 
observed a nonlinear growth of dunes. The flow measurements showed that the flow velocity 
in lobe region and turbulent kinetic energy in saddle region are increased. The mean sediment 
flux in the flow direction is directly proportional to the depth. Whereas, the turbulent fluxes 
exhibit an increasing trend up to 0.36–0.38 times the flow depth and then decrease with 
further increases in flow depth.

How to cite: Bodapati, S. S. P. and Chandra, V.: The Fractal and Topological Metrics for Assessing Three-Dimensionality in Dune Morphology , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18148, https://doi.org/10.5194/egusphere-egu25-18148, 2025.

EGU25-19135 | ECS | Orals | GM2.7

Quantifying Tidal Dune Morphodynamics at the Laboratory Scale: A Combined Measuring and Modelling Approach 

Gaetano Porcile, Dominique Mouazé, Pierre Weill, Aurélien Gangloff, and Anne-Claire Bennis

Understanding the morphodynamics of tidal dunes is essential for improving predictions of sediment transport and seabed evolution in coastal and estuarine environments. This study advances our understanding through a combined experimental and numerical investigation into the short-term morphodynamic evolution of laboratory-scale tidal dunes under controlled conditions.

Building on earlier flume experiments examining hydrodynamic interactions of reversing currents with fixed-bottom, sand-coated asymmetric compound dunes, we incorporated a cm-thick layer of unimodal sediment over the rigid dune models to simulate mobile-bed conditions. High-resolution Particle Image Velocimetry (PIV) was employed to capture detailed spatial and temporal dynamics of turbulent flows and the concurrent evolution of dune surfaces.

Complementary numerical modelling utilised the oceanographic circulation model CROCO, incorporating its non-hydrostatic solver and the USGS sediment transport module. The lab-scale model application was calibrated and validated against the laboratory measurements, demonstrating exceptional agreement in the short-term evolution of dune morphology. Key findings include the accurate replication of observed boundary layer dynamics, sediment transport mechanisms, and morphodynamic changes under reversing tidal currents. These experiments establish a solid benchmark for validating non-hydrostatic models of tidal dune morphodynamics.

This work underscores the transformative potential of integrating detailed physical experiments with advanced numerical models to refine our predictive capabilities for morphodynamic processes in tidal environments. The insights gained are particularly significant for coastal engineering and seabed mobility studies, with direct applications to the design and optimisation of offshore wind farm infrastructures.

How to cite: Porcile, G., Mouazé, D., Weill, P., Gangloff, A., and Bennis, A.-C.: Quantifying Tidal Dune Morphodynamics at the Laboratory Scale: A Combined Measuring and Modelling Approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19135, https://doi.org/10.5194/egusphere-egu25-19135, 2025.

EGU25-20382 | ECS | Orals | GM2.7

Submerged granular collapse: different cohesion strength and initial packing densities 

Rui Zhu, Zhiguo He, and Eckart Meiburg

We investigate the submerged cohesive collapse of cohesive granular columns, as a function of packing densities and cohesive force strength, via grain-resolving direct numerical simulations. We not only obtain the randomly packed granular columns but also the regular densely packed columns by Hexagonal close-packed (HCP) structure. The cohesive forces act to reduce the final runout distance of the collapsing column, which will no longer collapse when the cohesive force is larger than a critical value. This critical value decreases with the increase of the packing density. The cohesive forces significantly accelerate the contraction for loosely packed columns and decelerate the dilation for densely packed columns, resulting in a larger positive excess pore pressure and a smaller negative excess pore pressure, respectively. The collapsing column has distinct straight-like failure surfaces at the initial time, whose angle with the horizontal plane increases with the packing density. The force-chain network analysis indicates that the strong cohesive force chains form more easily in the failure region and have a larger size with increasing the cohesive force and packing density, which induces a larger macroscopic cohesive resistance. The cohesive force has a canceling effect on the normal contact force, which results in a smaller size for the contact force chains.

How to cite: Zhu, R., He, Z., and Meiburg, E.: Submerged granular collapse: different cohesion strength and initial packing densities, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20382, https://doi.org/10.5194/egusphere-egu25-20382, 2025.

EGU25-294 | Orals | ESSI4.11

Enhancing Forest Change Detection Using Self-Supervised Learning with Multi-Source EO Data 

Ridvan Kuzu, Antony Zappacosta, Oleg Antropov, and Octavian Dumitru

This study presents advancements in forest change detection by leveraging self-supervised learning (SSL) methods with multi-source and multi-temporal Earth Observation (EO) data. Transitioning from traditional bi-temporal approaches, the developed methodology incorporates multi-temporal analysis and multimodal data fusion using Sentinel-1, Sentinel-2, and PALSAR-2 imagery. Key innovations include mapping the magnitude of forest changes rather than binary classifications, enabling nuanced assessment of disturbance severity.

Experiments demonstrate the effectiveness of SSL-pretrained backbones, such as ResNet architectures, in extracting features for change detection. The integration of multi-temporal Sentinel-1 time series further improved the reliability and accuracy of disturbance tracking over time. These advancements show the potential of SSL to enhance forest change monitoring, providing scalable solutions for continuous and precise assessment of forest dynamics.

How to cite: Kuzu, R., Zappacosta, A., Antropov, O., and Dumitru, O.: Enhancing Forest Change Detection Using Self-Supervised Learning with Multi-Source EO Data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-294, https://doi.org/10.5194/egusphere-egu25-294, 2025.

Forest fragmentation disrupts habitat continuity, reshapes ecosystem processes, and threatens biodiversity. Effective conservation efforts in fragmented landscapes rely on precise monitoring of these changes. This study leverages remote sensing through vegetation indices to evaluate forest health and detect fragmentation-induced alterations over time. Focusing on the Tuchola Forest in Poland, an area increasingly affected by windstorms, we analyzed Sentinel-2 imagery from 2016 to 2024 using 19 vegetation indices. Machine learning classifiers—Extra Trees, Random Forest, and LightGBM—were employed to assess which indices best capture fragmentation stress. The Extra Trees classifier outperformed the others in accuracy and generalization, identifying NDWI and GNDVI as the most effective indicators. These indices were particularly responsive to shifts in vegetation water content and canopy density linked to fragmentation. Our findings underscore the utility of targeted vegetation indices for precise ecological monitoring and inform conservation strategies in fragmented forests.

How to cite: Dutt, S. and Kunz, M.: Uncovering Fragmentation Patterns: Optimal Vegetation Indices for Monitoring the Tuchola Forest Ecosystem, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-353, https://doi.org/10.5194/egusphere-egu25-353, 2025.

EGU25-670 | ECS | Orals | ESSI4.11

Integrating High-Resolution Thermal Mapping and Greenhouse Gas Emission Analysis for Climate Resilience in Urban, Peri-Urban and Rural Areas 

Naji El Beyrouthy, Mario Al Sayah, Rita Der Sarkissian, and Rachid Nedjai

Monitoring urban, peri-urban, and rural temperatures, along with greenhouse gas (GHG) emissions, is crucial for understanding local climate dynamics, especially in rapidly urbanizing areas. This study leverages advanced remote sensing techniques and environmental analysis to enhance high-resolution Land Surface Temperature (LST) mapping. It further investigates the relationship between LST and methane (CH₄) emissions - a significant driver of climate change - and their combined impact on Urban Heat Island (UHI) effects.

Leveraging multispectral atmospherically corrected imagery from LANDSAT 8-9 and SENTINEL-2 satellites, spectral harmonization techniques and Convolutional Neural Network (CNN)-based super-resolution models were applied to improve the spatial resolution and accuracy of LST calculation. These methods are further refined through the integration of key environmental indices, including soil characteristics, land cover, Normalized Difference Vegetation Index (NDVI), Normalized Difference Built-up Index (NDBI), and Normalized Difference Water Index (NDWI), which capture land use characteristics and their impact on thermal variations. The resultant LST at 1m was statistically validated against meteorological datasets by calculating Root Mean Squared Error and Mean Absolute Error, showing errors consistently below 2°C, with 75% of the values within 1°C. Making use of the accurate LST readings, air temperature (Ta) was derived using polynomial regression models, ultimately resulting in LST-derived air temperature maps with R² values exceeding 0.75.

Building upon this high-resolution thermal mapping, the study examines how agricultural zones are influenced by urban thermal dynamics exacerbated by GHG emissions creating a negative feedback loop where increased temperatures further impact agricultural practices and lead to additional GHG emissions. Seasonal and phenological variations in CH₄ emissions from major crops cultivated in the Loiret region including wheat, were analyzed. Results reveal that land use, crop phenology and soil characteristics significantly modulate LST, influencing both the intensity and distribution of urban heat anomalies. Moreover, the thermal contributions of these areas are analyzed within the context of their dual role. On one hand, these areas can act as potential moderators of UHIs by providing vegetative cover and cooling effects. On the other hand, they contribute to regional methane fluxes due to agricultural practices. This dual role highlights the complexity of peri-urban and rural zones, as they can simultaneously alleviate and exacerbate environmental challenges.

The presented framework can be considered as a contribution to bridging the gap between remote sensing advancements and climate science by providing actionable insights into the interactions between urban and rural thermal dynamics. The methodology not only offers a scalable approach for improving LST and Ta monitoring in data-sparse regions but also highlights the implications of land management practices for mitigating urban heat and reducing GHG emissions. By combining cutting-edge data processing techniques with environmental analysis, the study underscores the importance of integrating thermal mapping with greenhouse gas emission assessments to inform sustainable planning and climate adaptation strategies. In conclusion, this study contributes to the broader understanding of urban-rural thermal interdependencies and their role in shaping regional climate resilience, while also aiming to develop a new approach that leverages remote sensing to GHG emissions across wide areas.

How to cite: El Beyrouthy, N., Al Sayah, M., Der Sarkissian, R., and Nedjai, R.: Integrating High-Resolution Thermal Mapping and Greenhouse Gas Emission Analysis for Climate Resilience in Urban, Peri-Urban and Rural Areas, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-670, https://doi.org/10.5194/egusphere-egu25-670, 2025.

EGU25-1883 | ECS | Posters on site | ESSI4.11

Development of a Remote Crop Quality Sensor: Advancing Carotenoid Assessment with Raman Spectroscopy 

Miri Park, Annette Somborn, Dennis Schlehuber, and Volkmar Keuter

The accurate evaluation of crop quality is vital for sustainable agriculture and optimized production. Raman spectroscopy, renowned for its insensitivity to water interference and its ability to deliver molecular-specific information, presents significant potential as a remote sensing technology. This study explores the feasibility of adapting advanced Raman spectroscopy as a remote crop quality sensor for the precise assessment of carotenoids. Carotenoids were chosen due to their dual role as key stress indicators in crops and their well-established antioxidant benefits for human health.

To explore carotenoid variability, Arabidopsis thaliana and Spinacia oleracea were analyzed. Raman spectroscopy measurements were performed on two leaves per plant using a 785 nm laser. For the carotenoid quantification, Linear Discriminant Analysis (LDA) was adapted. The spectra were processed through smoothing, background removal, and normalization, followed by modification with an amplifying factor. This study evaluated the impact of these processing methods, particularly the application of the amplifying factor, on the accuracy of the model. High-Performance Liquid Chromatography (HPLC) was employed as the reference method for validation. Three-quarters of the samples were used to construct the model, while the remaining one-quarter was reserved for validation. As a result, the model utilizing spectra modified with the amplifying factor in most cases achieved higher validation accuracy compared to models based on unmodified spectra.

This study introduces a novel Raman spectroscopy-based remote sensing approach for crop quality assessment, establishing an enhanced model for interpreting spectral data. By enabling precise detection of stress-induced changes in plant chemical composition, including carotenoids, this technique paves the way for scalable, real-time monitoring through Raman-equipped machinery or drones, advancing sustainable agriculture practices.

How to cite: Park, M., Somborn, A., Schlehuber, D., and Keuter, V.: Development of a Remote Crop Quality Sensor: Advancing Carotenoid Assessment with Raman Spectroscopy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1883, https://doi.org/10.5194/egusphere-egu25-1883, 2025.

EGU25-1993 | Orals | ESSI4.11

Leveraging Satellite Earth Observation for Detecting Bloom Shifts and Phenological Patterns in California’s Almond Orchards 

Tarin Paz-Kagan, Oren Lauterman, Fadi Kizel, Maciej A. Zwieniecki2, Jessica Orozco, and Or Sperling

Given the impact of climate change on deciduous crop yields, our research focuses on leveraging earth observation remote sensing to accurately detect flowering periods in almond orchards and evaluate a climate-based dormancy model for predicting flowering times. This study addresses the challenge of monitoring almond flowering phenology by employing automated crop mapping techniques to support phenology monitoring across California's Central Valley. Using Sentinel-2 (S2) multispectral satellite imagery, we compare its effectiveness with the carbohydrate-temperature (C-T) dormancy model. The study area encompasses approximately 30,000 almond orchards, precisely identified using the Almond Industry Map. We utilized time-series analyses of the Enhanced Bloom Index (EBI) and the Normalized Difference Vegetation Index (NDVI) to quantify bloom periods and intensity and determine peak bloom times. Leveraging around 4,000 S2 tiles, enhanced vegetation indices, and in situ time-lapse camera data collected from 2019 to 2022, we developed a robust methodology for accurately identifying peak bloom periods. This process created a comprehensive phenological dataset, which was standardized and interpolated to daily resolution for improved time-series analysis. Our approach achieved a mean absolute error (MAE) of just 1.9 days in detecting peak bloom, demonstrating the accuracy of satellite-based phenological monitoring. This underscores both the advantages and limitations of remote sensing technologies in agricultural phenology. The dataset was then used to validate projections from the climate-based carbohydrate-temperature (C-T) dormancy model, offering valuable insights and supporting the refinement of this mechanistic approach. The study revealed significant spatial and temporal patterns in flowering phenology, emphasizing the role of regional climatic conditions in influencing crop development. Results highlight the potential of remote sensing and satellite imagery to detect the start, peak, and end of bloom in almond orchards with high precision, generate valuable phenological datasets, monitor patterns at both regional and field scales, and assess the reliability of dormancy models. This research has critical implications for improving agricultural practices and supporting decision-making in the almond industry. By advancing phenological monitoring techniques, our study presents a scalable and innovative approach to managing perennial crops in the face of climate change.

How to cite: Paz-Kagan, T., Lauterman, O., Kizel, F., Zwieniecki2, M. A., Orozco, J., and Sperling, O.: Leveraging Satellite Earth Observation for Detecting Bloom Shifts and Phenological Patterns in California’s Almond Orchards, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1993, https://doi.org/10.5194/egusphere-egu25-1993, 2025.

Selecting the appropriate unmanned aerial vehicle flight height is beneficial for increasing the monitoring efficiency. We firstly used an unmanned aerial vehicle to explore the scale effect on monitoring rice aboveground biomass. The results confirmed the feasibility of using vegetation indices and textures from hyperspectral images to improve the estimations at different spatial resolutions. The monitoring accuracy of combining vegetation indices and textures was the highest, and exhibited a decreasing trend as the spatial resolution decreased with the greatest accuracy appearing at 13 cm. Two new concepts were proposed: “appropriate monitoring scale domain” to define the range of spatial resolution where the monitoring accuracy was less affected by scale effect, and “appropriate monitoring scale threshold” to define the spatial resolution where accuracy dropped noticeably. The appropriate monitoring scale domains varied at different growth stages and the appropriate monitoring scale thresholds of using vegetation indices and textures were lower than those using textures: 39 cm, 52 cm, and 65 cm at the pre-heading, post-heading, and entire growth stages, respectively when using textures, and 52 cm, 65 cm, and 78 cm at the corresponding growth stages when combining vegetation indices and textures. In terms of aboveground biomass level, growth stage and error value, the relatively lower aboveground biomass levels, earlier growth stages of the multi-temporal models, and overestimations were more likely to yield notable accuracy changes when the spatial resolution converted to lower level on both sides of appropriate monitoring scale threshold. Vegetation indices containing red-edge or near-infrared bands were effective for estimation. Yellow/green band textures and vegetation indices containing green bands with near-infrared/red-edge bands also obtained inspiring performances. MEA was indispensable in estimation while more diverse textures were incorporated into the models of the entire growth stages and models established at lower spatial resolutions. These findings are essential for understanding the scale effect in estimating rice aboveground biomass, facilitating efficient monitoring at field scale.

How to cite: Xu, T., Wang, F., and Shi, Z.: Multi-scale monitoring of rice aboveground biomass by combining spectral and textural information from UAV hyperspectral images, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2093, https://doi.org/10.5194/egusphere-egu25-2093, 2025.

EGU25-2120 | ECS | Orals | ESSI4.11

A new framework for mapping time series rubber plantation in Southeast Asia 

Yaoliang Chen and Hongfeng Xu

Accurate yield estimation and appropriate planting management policies for rubber plantations require their precise information on spatiotemporal change data. Previous studies on mapping of rubber plantations did not employ the dynamic rubber phenology features and had difficulty in obtaining historical samples. Here we attempted to develop a new mapping framework through taking historical sample migration, dynamic phenology, and change detection variables into the classification procedure. An automatic sample migration algorithm was first proposed to generate historical samples. Then, two new variable types, dynamic phenology indices and change detection variables, were developed. Another four commonly used variable types -spectral bands, yearly composite spectral indices, terrains, and textures were also extracted. Five combinations of variable types were designed to explore key variable types. Subsequently, the framework with recommended variable types was applied at an experimental site in China and was finally evaluated to two test sites in Myanmar and Thailand for examining its transferability. Results showed that the average overall accuracy of historically migrated samples reached over 97% at the experimental site. Dynamic phenology indices and change detection variables were found as two crucial variable types for rubber plantations mapping. The average rubber plantations mapping accuracy during 2003-2022 reached 93.68%. Transferring the proposed framework to two test sites confirmed the independent roles of change detection variables and dynamic phenology indices. Their average rubber plantations mapping accuracy during 2003-2022 reached 94.34% and 93.73%, respectively. Good spatial consistency between the classified maps and Google Earth images was observed, displaying clear boundaries between rubber plantations and farmland, evergreen broadleaf forest, and shrub. Overall, the proposed framework has great potential for time series rubber plantations mapping in Southeast Asia.

How to cite: Chen, Y. and Xu, H.: A new framework for mapping time series rubber plantation in Southeast Asia, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2120, https://doi.org/10.5194/egusphere-egu25-2120, 2025.

The snow cover occurrence index (SCOI), deffned as the ratio of the number of times that a pixel is classiffed as snow to the number of times that the pixel is observed in optical remote sensing data over a given year, can effectively mitigate the inffuence of clouds and holds great potential for extracting the annual snow duration and glacier extent in mountainous regions. The SCOI of the Qinghai–Tibet plateau (QTP) is calculated and analyzed on the basis of Landsat images from 1985 to 2021. The results indicate the following: 1) the evaluation based on station snow depth reveals that the SCOI is stable when the number of combined years reaches 5; 2) the SCOI has a strong correlation with snow cover days (SCD) determined from Moderate Resolution Imaging Spectroradiometer (MODIS) snow cover products; and 3) the SCOI has good potential for glacier extraction and exhibits a high level of consistency with glacier boundary survey data. Overall, owing to the higher spatial resolution and longer duration of the Landsat-based SCOI, it can accurately describe the distribution characteristics and changes in snow cover and glaciers in complex mountainous areas. 

How to cite: Wang, X.: A Novel Snow Cover Occurrence Index (SCOI) for the Dynamics of Snow Duration and Glacier Extent in Mountainous Regions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2205, https://doi.org/10.5194/egusphere-egu25-2205, 2025.

EGU25-2520 | ECS | Orals | ESSI4.11

Linking Citrus Fruit Cracking Intensity to Plant Water Status: Insights from UAV-Derived Metrics Validated by Ground-Based Data 

Moshe (Vladislav) Dubinin, Michael Morozov, Avi Sadka, and Tarin Paz-Kagan

Citrus fruit cracking, a physical failure of the peel, causes yield losses of 10% to 35%, peaking during October-November. Water status of the tree and water flow into the fruit influence this phenomenon. with excessive irrigation during critical fruit development stages exacerbates cracking. As part of the EU-Horizon CrackSense project, this study is aimed to link citrus tree plant water status (PWS) to fruit cracking, emphasizing how deficit irrigation can reduce yield loss due to cracking. Using UAV and eco-physiological measurements, we developed models to predict PWS and its relationship with cracking intensity early in the season. The study, conducted in 2023-2024 in a commercial orchard near Kfar Chabad, Israel, tested four irrigation treatments: control, defined as the standard irrigation, two deficits irrigations regimes (50% of control) early and late in the season, and excessive irrigation (150% of control) throughout the season. Ground-based measurements included fruit and trunk diameter, stem water potential (SWP), stomatal conductance, plant area index (PAI), and growth rate (TG). UAV flights integrated multispectral, thermal, and LiDAR sensors to capture spatial-temporal variability in PWS. Canopy metrics, such as height, volume, LiDAR-based PAI, and spectral and thermal indices, were incorporated into PWS models. Results revealed significant differences in TG, SWP, and stomatal conductance for 50% of early and late deficit irrigation treatments compared to other treatments. Random forest models demonstrated strong predictive performance for SWP (R² > 0.77) and TG (R² > 0.76). LiDAR-derived PA correlated highly with field optical measurements (R² = 0.92), yield (R² = 0.67), and cracked fruit percentages (R² > 0.50). This study underscores the importance of precise irrigation management in reducing fruit cracking. It highlights the potential of remote sensing systems for predicting cracking and managing water status at the tree level. The developed models equip farmers with tools to apply controlled water stress, minimizing cracking and improving yield.

How to cite: Dubinin, M. (., Morozov, M., Sadka, A., and Paz-Kagan, T.: Linking Citrus Fruit Cracking Intensity to Plant Water Status: Insights from UAV-Derived Metrics Validated by Ground-Based Data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2520, https://doi.org/10.5194/egusphere-egu25-2520, 2025.

EGU25-2532 | Orals | ESSI4.11

Cross-Year Crop Mapping with Thermal Calendar from Optical Satellite Image Time Series 

Mehmet Ozgur Turkoglu and Helge Aasen

Traditional approaches for crop type classification from optical satellite images typically evaluate algorithms using training and test datasets from the same year and based on calendar days. However, this experimental setup is not practical for real-world applications due to (i) year-to-year variations in crop growth caused by climate, which limit generalization, and (ii) the inability to apply a model to the current year if trained on current-year data. This work addresses these challenges by introducing a cross-year experimental setting and incorporating thermal calendars into our deep learning model. Specifically, we train an attention-based deep learning model on the 2021 Swiss crop dataset, validate it in 2022, and test it in 2023. Thermal calendars, derived from accumulated daily average temperatures, align crop growth with thermal time instead of calendar time, addressing temporal shifts caused by climatic variations. Our results demonstrate that integrating thermal calendars improves performance compared to baseline using standard calendar encodings, achieving better generalization across years and showcasing the potential for large-scale operational crop classification.

How to cite: Turkoglu, M. O. and Aasen, H.: Cross-Year Crop Mapping with Thermal Calendar from Optical Satellite Image Time Series, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2532, https://doi.org/10.5194/egusphere-egu25-2532, 2025.

EGU25-2602 | ECS | Orals | ESSI4.11

LiDAR-based indices and machine learning efforts to model biophysical estimations of corn (Zea mays L.) 

K. Colton Flynn, Gurjinder Baath, Bala Ram Sapkota, and Douglas R. Smith

Light Detection and Ranging (LiDAR) in precision agriculture is gaining traction as the technology becomes both accessible and affordable, particularly for assessing biophysical characteristics of vegetation. This study investigates the potential of unmanned aerial vehicle (UAV)-based LiDAR data for modeling Leaf Area Index (LAI), a key indicator of crop health and productivity. We explore laser penetration indices to model LAI and compare these results with machine learning models using various LiDAR return types (e.g., ground, vegetation, first, last). In both approaches, in-situ LAI measurements obtained with a LiCOR LAI-2000 were used as ground truth. The study was conducted over two years with a multi-date planting of corn (Zea mays L.) in Temple, TX. Our findings indicate that LiDAR-based methods, both through penetration indices and machine learning, hold promise for accurately modeling LAI and other biophysical crop traits in precision agriculture.

How to cite: Flynn, K. C., Baath, G., Sapkota, B. R., and Smith, D. R.: LiDAR-based indices and machine learning efforts to model biophysical estimations of corn (Zea mays L.), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2602, https://doi.org/10.5194/egusphere-egu25-2602, 2025.

Bananas are the tropical fruit with the largest global cultivation area, sales volume, and 
international trade. China is the world's second-largest producer and consumer of bananas. 
Rapid and accurate acquisition of banana planting range and spatial distribution information 
is crucial for promoting the sustainable development of the banana industry in China. 
Currently, research on banana classification and identification faces challenges such as 
insufficient mechanistic understanding, poor generalizability, and difficulties in large-scale 
application. Additionally, banana cultivation areas are often located in regions with cloudy 
and rainy climates, limiting the acquisition of optical imagery. To address this, this study 
constructs a banana identification model based on phenological characteristics: (1) Sentinel
1/2 imagery is utilized to obtain time series curves of banana spectral and scattering features, 
followed by interpolation and filtering of the time series data; (2)A phenological index based 
on optical and scattering features is developed according to banana phenological 
characteristics. By combining SAR with the index, the model's mechanistic understanding is 
enhanced while alleviating the challenges posed by cloud cover in tropical and subtropical 
regions; (3)Using the constructed phenological index alongside banana spectral, texture, and 
temporal features, a classification model is trained for banana identification in the study area. 
This banana forest identification model and the developed phenological index aim to resolve 
current issues in banana classification and provide theoretical and practical support for large
scale banana extraction and the study of tropical and subtropical economic crops.

How to cite: wang, Z.: Banana plantation identification using remote sensing data in tropical and subtropical regions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2709, https://doi.org/10.5194/egusphere-egu25-2709, 2025.

EGU25-4248 | Orals | ESSI4.11

Characterisation and Calibration of Low-Cost IoT Monitoring Systems for Extreme Environmental Conditions  

Laura Mihai, Cristina Toma, Razvan Mihalcea, Karolina Sakowska, Loris Vescovo, Luca Belelli Marchesini, Valerio Coppola, Francesco Renzi, and Riccardo Valentini

Monitoring forests in hard-to-reach locations and under extreme climatic conditions requires reliable, long-term data collection systems. Low-cost devices are increasingly being developed for this purpose; however, deploying these systems without thorough characterisation and calibration can compromise data quality. This work emphasises the importance of fully characterising and calibrating such systems prior to installation to ensure accuracy and reliability over extended periods. This study was conducted as part of the RemoTrees project, which aims to develop a unique IoT tree monitoring system equipped with satellite communication and designed to withstand extreme environmental conditions. A set of the alpha version prototypes, developed within the project, was evaluated in this work. The evaluation focused mainly on a set of low-cost environmental monitoring devices equipped with radiometric sensors measurements. The key performance parameters were assessed, including signal-to-noise ratio (SNR), irradiance sensor detector nonlinearity, sensitivity to temperature variations, and angular response influenced by the diffusive optics. Each parameter was analysed to determine system performance under close to real-world conditions, using both laboratory and in situ validation setups. Key findings revealed that without proper optics used the accuracy of irradiance measurements are significantly influenced. Improvements on the system design and on calibration procedures were implemented to address these issues, improving the overall accuracy and stability of the systems. By addressing these challenges, the systems demonstrated enhanced robustness and suitability for long-term environmental monitoring in extreme conditions. This study underscores the necessity of rigorous pre-deployment testing and calibration for low-cost monitoring devices, particularly when deployed in challenging environments. The findings contribute to advancing the development and deployment of cost-effective technologies for environmental monitoring, enabling more sustainable and accessible data collection practices in forests under extreme climatic conditions.

How to cite: Mihai, L., Toma, C., Mihalcea, R., Sakowska, K., Vescovo, L., Marchesini, L. B., Coppola, V., Renzi, F., and Valentini, R.: Characterisation and Calibration of Low-Cost IoT Monitoring Systems for Extreme Environmental Conditions , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4248, https://doi.org/10.5194/egusphere-egu25-4248, 2025.

EGU25-4513 | ECS | Orals | ESSI4.11

A Machine Learning-based Surrogate Model for Optimization of Cropping Systems in Denmark 

Meshach Ojo Aderele, Edwin Haas, Klaus Butterbach-Bahl, and Jaber Rahimi

Process-based agricultural system models (PBMs) are pivotal tools for evaluating the environmental impacts of agricultural practices. However, their large-scale application is constrained by significant computational demands, extensive time requirements, and data availability. These challenges hinder policymakers and land managers in implementing sustainable agricultural practices at scales meaningful for decision-making. Recent advancements in machine learning (ML) offer a promising solution by providing computationally efficient alternatives, yet the lack of interpretability regarding agro-environmental processes remains a critical barrier.

In this study, we address this challenge by developing a machine learning-based surrogate model for LandscapeDNDC (LDNDC) framework. The surrogate model predicts key agro-environmental variables, including yield, nitrous oxide (N2O) emissions, nitrate leaching (NO3-), and soil organic carbon (SOC), at a national scale for Denmark. Synthetic data were generated using a factorial design based on observed crop practices in Denmark, utilizing field-level data collected across six Danish catchments between 2013 and 2019 as part of the National Monitoring Program for Water Environment and Nature (NOVANA; LOOP-program). This approach incorporated crop rotations as well as spatially disaggregated information on soils and weather, resulting in a dataset comprising approximately 2 billion rows. To enhance the dataset's versatility and account for potential future scenarios, factors like manure amount and synthetic fertilizer amount were extrapolated beyond its current observed ranges. The synthetic dataset was subsequently simulated using the LDNDC modelling framework, and the resulting outputs were employed to train a variety of machine learning algorithms utilizing multi-task learning, optimizing predictions for multiple agro-environmental variables of interest.

Our results demonstrate that the ML-based surrogate model not only significantly reduces computational cost and processing time but also enables the exploration of multiple cropping scenarios with greater efficiency. This approach facilitates rapid scenario testing and optimization, making it accessible to policymakers and farmers without the constraints imposed by traditional PBM frameworks. We propose this methodology as a scalable and practical tool for advancing sustainable agricultural decision-making.

How to cite: Aderele, M. O., Haas, E., Butterbach-Bahl, K., and Rahimi, J.: A Machine Learning-based Surrogate Model for Optimization of Cropping Systems in Denmark, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4513, https://doi.org/10.5194/egusphere-egu25-4513, 2025.

EGU25-4726 | ECS | Posters on site | ESSI4.11

Combining geometric-optical and spectral invariants theories for modeling canopy fluorescence anisotropy 

Yachang He, Yelu Zeng, and Dalei Hao

The spectral invariants theory (p-theory) has received much attention in the field of quantitative remote sensing over the past few decades and has been adopted for modeling of canopy solar-induced chlorophyll fluorescence (SIF). However, the spectral invariant properties (SIP) in simple analytical formulas have not been applied for modeling canopy fluorescence anisotropy primarily because they are parameterized in terms of leaf total emissions and scatterings, which precludes the differentiation between forward and backward leaf SIF emissions. In this study, we have developed the canopy-SIP SIF model by combining geometric-optical (GO) theory to account for asymmetric leaf SIF forward and backward emissions at the first-order scattering and by modeling multiple scattering based on the p-theory, thus avoiding the dependence on radiative transfer models. The applicability of the model simulations especially over 3D heterogeneous canopies was improved by incorporating canopy structure through multi-angular clumping index, and by modeling single scattering from the four components of the scene in view according to the GO approach. The results show good consistency with both the state-of-the-art SIF models and multi-angular field SIF observations over grass and chickpea canopies. The coefficient of determination (R²) between the simulated SIF and field measurements was 0.75 (red) and 0.74 (far-red) for chickpea, and 0.65 (both red and far-red) for grass. The average relative error was approximately 3% for 1D homogeneous scenes when comparing the canopy-SIP SIF model simulations to the SCOPE model simulations, and around 4% for the 3D heterogeneous scene when comparing to the LESS model simulations. The results indicate that the proposed approach for separating asymmetric leaf SIF emissions is a robust way to keep a balance between satisfactory simulation accuracy and efficiency. Model simulations suggest that neglecting the leaf SIF asymmetry can lead to an underestimation of canopy red SIF by 16.1% to 43.4% for various canopy structures. This study presents a simple but efficient analytical approach for canopy fluorescence modeling, with potential for large-scale canopy fluorescence simulations.

How to cite: He, Y., Zeng, Y., and Hao, D.: Combining geometric-optical and spectral invariants theories for modeling canopy fluorescence anisotropy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4726, https://doi.org/10.5194/egusphere-egu25-4726, 2025.

EGU25-4910 | ECS | Orals | ESSI4.11

Mapping 10-m monoculture and intercropped maize of Kenya with phenology knowledge and Sentinel-2 data 

Yang Chen, Lijun Zuo, Xianhu Wei, Xiao Wang, and Jinyong Xu

In East Africa, lack of agriculture inputs and unstable climates lead to 50% yield gaps, making intercropping—the planting of more than one crop in the same parcel of land—a common agricultural management practice among smallholder farmers to improve land-use efficiency and reduce risks. In Kenya, where maize is the staple food, maize is often intercropped with beans, legumes, and potatoes. Despite its widespread, agricultural statistics on intercropping are currently sparse, and remote sensing approaches for large-scale crop monocultures are often unsuitable for intercropping monitoring. Mapping intercropping at national scale is extremely challenging because of heterogeneous landscapes, lack of cloud-free satellite imagery, and the scarcity of high-quality ground-based situ data in these regions. This study addressed these challenges using a phenology-assisted automated mapping framework on Google Earth Engine (GEE) to create 10m-resolution maps of monoculture and intercropped maize across Kenya for the long and short rainy seasons of 2023.
First, we computed 10-day median composites of Sentinel-2 optical reflectance data for each pixel in the region to build monoculture/intercropped/non-maize Random Forest (RF) classifiers. Several thousand crop ground labels were collected during field surveys in 2023, including monoculture maize (mono-maize), intercropped maize (in-maize), and other crops (e.g., wheat, rice, coffee, tea, sugarcane, potatoes, beans, etc.). To address the limited availability of intercropped maize samples, a novel phenology-based approach was implemented. Maize was first differentiated from other crops by analyzing TCARI and OSAVI during the vegetative phase and ARI during maturity. Additionally, lower greenness and moisture levels in intercropped systems, which have larger planting width and more short-term crops, were detected using the SWIR1/NDVI ratio, effectively distinguishing mono-maize from in-maize. Automatically derived monoculture/intercropped maize samples and 40% of ground samples were used for training, while the remaining ground data were used for accuracy assessment. 
For the long rainy season, the overall accuracy (OA) was 0.88, with an F1-score of 0.87 for mono-maize and 0.78 for in-maize. For the short rainy season, OA dropped to 0.85, with F1-scores of 0.82 for mono-maize and 0.72 for in-maize. Misclassification primarily arose from phenological similarities between mono-maize and in-maize and increased planting of other crops with similar patterns during the short rainy season. Results revealed that 854,432 hectares of mono-maize were concentrated in the Western region and Rift Valley plateau during the long rainy season, while 1,061,701 hectares of in-maize were widely distributed across the region, particularly near Mount Kenya and the Eastern region. In the short rainy season, reduced and erratic precipitation led to decreased maize planting, with more farmers opting for intercropped systems and short-term crops to reduce risks of crop failure. 
We are convinced that this study is a crucial first step to demonstrate the potential of Sentinel-2 data and phenology-based automated mapping for large-scale monitoring of intercropping, providing critical insights for agricultural monitoring in sub-Saharan Africa. It serves as a foundation for developing a regional archive of monoculture and intercropped crop systems and addressing key agricultural challenges across the region.

How to cite: Chen, Y., Zuo, L., Wei, X., Wang, X., and Xu, J.: Mapping 10-m monoculture and intercropped maize of Kenya with phenology knowledge and Sentinel-2 data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4910, https://doi.org/10.5194/egusphere-egu25-4910, 2025.

A study conducted in a northern Jordanian arid Mediterranean grassland between 2017 and 2021 examined the relationship between remotely sensed Normalized Difference Vegetation Index (NDVI) and modeled standing crop biomass. The research sought to determine the utility of high-resolution (10-meter) Sentinel-2 imagery, coupled with the PHYGROW model, for biomass estimation in this challenging environment, and to assess the potential of NDVI as a cost-effective alternative to traditional ground-based methods. Data were aggregated into 10-day intervals for temporal analysis. Results indicated a significant positive correlation (p < 0.001) between NDVI and standing crop (kg/ha), described by the linear model: Standing crop = 60.40 + 3567.56 × NDVI (R² = 0.52). This finding suggests that NDVI offers a reliable and time effective approach to biomass estimation in such settings.

The strong positive correlation between NDVI and standing crop highlights the potential of remote sensing for large-scale rangeland health monitoring. Tracking NDVI changes over time provides insight into vegetation responses to climate, grazing, and conservation efforts. This understanding supports decision-making for sustainable grazing, water management, and conservation strategies. Future research should validate these findings on larger scales and explore integrating NDVI with other data, like soil moisture, to refine predictive models and improve accuracy. The study advocates adopting NDVI-based monitoring in arid rangeland management.

How to cite: Alhamad, M. N.: Integrating Sentinel-2 Imagery and PHYGROW Model for Biomass Estimation in Arid Rangelands of Northern Jordan, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5178, https://doi.org/10.5194/egusphere-egu25-5178, 2025.

EGU25-5892 | ECS | Orals | ESSI4.11

Assessment of bud flush and damage in young Norway Spruce trees through airborne high-resolution multispectral images 

Louisa Eurich, Sara López Fernández, Malin Elfstrand, María Rosario García-Gil, Jonas Bohlin, and Eva Lindberg

Scandinavia is facing climate changes with a predicted increase in mean temperature of 2-4°C. For Swedish forests to be adapted to this challenge, the Swedish tree breeding program aims to select trees that are adapted to different biotic and abiotic conditions. Information on spring phenology, damage and vitality are important variables in the Norway spruce selection process. Traditionally, the data is gathered through manual assessment of each tree, which requires significant resources and limits the number and frequency of variables that can be measured. As an alternative, Remote Sensing is a promising technology to evaluate bud flush and vitality in conifers, offering the advantage of scoring more trees in a shorter time with fewer resources while obtaining data for several time points during the vegetation season, and its use of algorithms to measure variables reduces the risk of human error.

This project aims to develop methods that can be used within the breeding program by collecting information on spring phenology, damage and vitality using high-resolution multispectral drone images of young Norway spruce trees. Data were collected during spring 2023 and 2024. Bud flush is estimated from the spectral values of the tree crowns using manual assessment of the flush in a subset of the trees as training data. The high-resolution multispectral images will also be used to assess the damage and vitality of the new shoots. To ensure capturing the bud flush at a high temporal resolution, images were taken before the vegetation season and up to twice weekly during the period with the most rapid flush. In the final step, the spatial pattern within the study sites will be analyzed and connected to damage and vitality of the young Norway Spruce trees.

 

How to cite: Eurich, L., López Fernández, S., Elfstrand, M., García-Gil, M. R., Bohlin, J., and Lindberg, E.: Assessment of bud flush and damage in young Norway Spruce trees through airborne high-resolution multispectral images, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5892, https://doi.org/10.5194/egusphere-egu25-5892, 2025.

EGU25-5987 | ECS | Posters on site | ESSI4.11

Soil Moisture Retrieval Over Agricultural Fields Using Synthetic Aperture Radar (SAR) Data 

Nguyen-Thanh Son, Chi-Farn Chen, Cheng-Ru Chen, Yi-Ting Zhang, Shu-Ling Chen, and Shih-Hsiang Chen

Soil moisture is vital for agricultural fields as it determines water availability for crops, directly affecting plant growth and productivity. It regulates nutrient uptake, root development, and microbial activity, ensuring efficient use of fertilizers and soil resources. Proper soil moisture levels prevent water stress, reduce crop failure risks, and optimize water irrigation efficiency. Accurate soil moisture monitoring supports sustainable farming practices, helps mitigate drought impacts, and enhances climate resilience. By maintaining optimal soil moisture, farmers can improve resource use, boost crop yields, and promote long-term agricultural sustainability. This study aims to develop an approach for retrieving soil moisture from Sentinel-1 A Synthetic Aperture Radar (SAR) data. The SAR data were processed for the 2024 dry season using a triangle-based approach in the Mekong Delta, Vietnam, following three main steps: (1) data preprocessing to convert raw radar backscatter values into the sigma naught (σ₀) backscatter coefficient in decibels (dB). This involves radiometric calibration, noise removal, and logarithmic scaling to enhances data interpretability, allowing for better comparisons across different radar acquisitions and improved analysis accuracy, (2) soil moisture retrieval by means of a triangle-based method developed based on the dual-polarization modes of the vertical transmit and vertical receive polarization (VV) and vertical transmit and horizontal receive polarization (VH). This method employs the triangular feature space created by using change in VV backscatter coefficients and the radar vegetation index (RVI), in which RVI helps distinguish vegetation effects while VV backscatter provides information on soil moisture. Combining both parameters thus allows for more precise moisture estimation even in complex environments, and (3) error verification. The results of soil moisture retrieval compared with the reference data showed moderate positive correlation, with the values of correlation coefficient (r) greater than 0.5 and the root mean square error (RMSE) smaller than 0.05, respectively. The lower soil moisture levels were especially observed in coastal areas, where higher evaporation rates, saline intrusion, and limited rainfall contribute to drier soils. These conditions create challenges for agriculture in coastal regions, as crops are more susceptible to drought stress and water shortages. Consequently, managing soil moisture becomes crucial for maintaining crop productivity and ensuring sustainable farming in coastal provinces. Eventually, soil moisture data was spatially aggregated with cropping areas to improve management practices in the region, allowing precise monitoring of soil conditions relative to specific crops and enabling tailored irrigation and water management strategies. This approach, leveraging dual-polarization SAR data with aid of the triangle-based method, could enhance soil moisture monitoring in agriculture and is completely transferable to other regions across the globe for soil moisture monitoring.

How to cite: Son, N.-T., Chen, C.-F., Chen, C.-R., Zhang, Y.-T., Chen, S.-L., and Chen, S.-H.: Soil Moisture Retrieval Over Agricultural Fields Using Synthetic Aperture Radar (SAR) Data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5987, https://doi.org/10.5194/egusphere-egu25-5987, 2025.

EGU25-6071 | Orals | ESSI4.11

Sensor Spatial Planning Methodology for Optimal Coverage and Data Accuracy in Agricultural Parcels 

Efthymios Papachristos, Marios Vlachos, and Angelos Amditis

Accurate sensor placement is critical in precision agriculture to collect high-resolution data essential for effective monitoring and decision-making. This study presents a comprehensive methodology for optimizing the spatial placement of sensors, focusing on determining the number of sensors needed and their optimal positions to ensure data quality and adequate area coverage. This methodology addresses the challenges posed by terrain restrictions, cost constraints, and data resolution needs. It is versatile, supporting in-situ monitoring, UAV-based sensing, and soil sampling for applications such as soil health analysis and soil organic carbon prediction models.

In many Research and Innovation Labs (RILs), the resolution of Earth Observation (EO) data, such as Sentinel-5 imagery with a resolution of 5×3 km, is often insufficient for the specific needs of agricultural parcels. To complement EO data, additional information must be gathered using in-situ sensors or UAVs. These additional data collection methods can provide higher resolution and more diverse data types, which are crucial for localized agricultural applications. However, the placement of sensors significantly impacts the quality and adequacy of the collected data. Dense sensor deployment across an entire area is often infeasible due to terrain challenges, budgetary limits, and the specific nature of the data being collected.

The methodology developed to address these challenges combines convex optimization, soft clustering, and cost-minimization techniques. The process begins by analyzing the statistical properties of the dataset, such as maximizing variance and maintaining the mean value, to ensure comprehensive data representation. This approach identifies key locations within the parcel that can adequately describe distributed values, reducing the need for excessive sensor deployment while maintaining data integrity.

For areas with existing spatial maps or datasets, the methodology applies weighted subsampling and soft clustering to identify optimal sensor locations. Weighted distributions prioritize critical areas for data collection, ensuring that key zones receive sufficient coverage. In cases where spatial maps are unavailable, an in-house cost-minimization algorithm guides the placement of sensors or UAVs. This algorithm incorporates factors such as terrain, accessibility, and installation costs to balance logistical constraints with data coverage requirements.

This methodology is compatible with diverse data sources, including EO data, hyperfield data, and in-situ sensor data from IoT networks. For instance, it can leverage data from soil moisture monitoring systems. Additionally, the methodology can guide soil sampling strategies for soil health assessment and serve as input for soil organic carbon prediction models. Its adaptability allows it to meet the needs of various agricultural monitoring applications, ranging from broad-scale field evaluations to detailed soil property studies.

Moreover, it enhances data quality by ensuring optimal sensor placement that captures maximum variability within the monitored area and it reduces costs and improves efficiency by minimizing the number of sensors needed. The approach is scalable and flexible, accommodating parcels of varying sizes and adapting to different data collection requirements and its integration with multiple data sources provides a comprehensive and cost-effective solution for advancing precision agriculture and sustainable resource management.

Acknowledgement:

This research has been funded by European Union’s Horizon Europe research and innovation programme under ScaleAgData project (Grant Agreement No. 101086355).

How to cite: Papachristos, E., Vlachos, M., and Amditis, A.: Sensor Spatial Planning Methodology for Optimal Coverage and Data Accuracy in Agricultural Parcels, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6071, https://doi.org/10.5194/egusphere-egu25-6071, 2025.

EGU25-6085 | Orals | ESSI4.11

Integrating UAV Multispectral Data into a Combined Crop-Radiative Transfer Model for Processing Tomatoes Using a Particle Filter 

Amit Weinman, Nitzan Malachy, Raphael Linker, and Offer Rozenstein

The proliferation of remote sensing (RS) data and advancements in mechanistic crop modeling and data assimilation techniques necessitate a framework that digitally represents cropping systems and their spectral properties. Such a framework would enable crop growth simulation, scenario testing, and timely prediction updates using RS data.

In this study, we develop a comprehensive coupling scheme that links a crop model (DSSAT-CROPGRO) with a radiative transfer model (RTMo module in SCOPE). This integration allows for the utilization of reflectance data from all measured spectral bands during data assimilation (DA) into the crop model.

We apply this coupled crop-radiative-transfer model in a DA experiment using a novel particle filter scheme. The assimilated data consists of observed reflectance measurements obtained by a multispectral camera mounted on an unmanned aerial vehicle (UAV). Using multispectral data with a high spatial resolution for analyzing a row crop required a dedicated analysis to fit model simulations to measurements. The suggested DA scheme was implemented in an irrigation and fertilization trial with processing tomatoes to evaluate its effectiveness.

The results showed that applying the DA scheme improved the NRMSE of the Leaf Area Index (LAI) from 59% to 41.8% and yield from 63.6% to 35.4%. The DA scheme performed best when the treatment that included the most severe stress was excluded from weight calculation, resulting in NRMSE of 34.1% and 15.5% for LAI and yield, respectively. After showing promising results, the suggested data assimilation scheme should be tested in large-scale, commercial fields using space-borne RS data to examine its applicability in various scenarios.

How to cite: Weinman, A., Malachy, N., Linker, R., and Rozenstein, O.: Integrating UAV Multispectral Data into a Combined Crop-Radiative Transfer Model for Processing Tomatoes Using a Particle Filter, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6085, https://doi.org/10.5194/egusphere-egu25-6085, 2025.

EGU25-6149 | ECS | Posters on site | ESSI4.11

UAV-based disease and pest detection using AI: Time to reconsider our approach? 

Eline Eeckhout, Pieter Spanoghe, and Wouter Maes

Rapid advancements in technology, particularly the rise of artificial intelligence (AI) and the integration of uncrewed aerial vehicles (UAVs) equipped with RGB, multi- and hyperspectral sensors, have boosted agricultural research on crop disease detection. This has led to a surge in studies exploring high-technology approaches to detecting crop diseases. While numerous studies have demonstrated high accuracy in detecting specific diseases or pests in crops, concerns arise regarding their reproducibility and generalisability.

We conducted a meta-analysis of over 100 research papers to examine how models are trained and validated, with a focus on how datasets for training, validation and testing were handled. In principle, a model can only be considered robust and widely applicable if it performs well on an entirely new dataset, i.e., a dataset it wasn’t specifically trained one. Otherwise, AI models risk overfitting to specific datasets or fields, potentially detecting signals that are not universal or not related to the targeted pest or disease. This issue arises when datasets are randomly split in training, validation and test subsets.

Our analysis revealed significant limitation in current practices. Nearly half of the reviewed papers relied on a single dataset (one single field, one single flight) for both model training and validation. About one-quarter of the studies used data from a single field with repeated flights during the same growing season. Only another quarter utilized datasets from multiple fields; however, the majority of these studies still used a random split for training and testing, meaning their models were not evaluated on independent datasets. In addition, a handful of studies using RGB data, applied transfer learning, with models pretrained on public (non-UAV) datasets and then applied to UAV datasets.

Overall, only 10% of the reviewed papers validated their models on fully independent datasets, i.e, using transfer learning or using an independent (untrained) separate field to test the model. We found that particularly models constructed with multispectral or hyperspectral data did not use independent datasets. On top of that, none of the studies explicitly tested whether their models were pest- or disease-specific, i.e., whether the models were sensitive only to the pest or disease they were trained to detect.

These findings highlight a critical limitation in the robustness and scalability of current AI-approaches to crop disease detection with UAVs. To address this, we call on researchers to include independent test datasets in their studies, and urge journals and reviewers to prioritize this criterion during evaluations. Additionally, we advocate for the public sharing of datasets to enable the development of robust and generalisable methods.

How to cite: Eeckhout, E., Spanoghe, P., and Maes, W.: UAV-based disease and pest detection using AI: Time to reconsider our approach?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6149, https://doi.org/10.5194/egusphere-egu25-6149, 2025.

EGU25-6243 | ECS | Posters on site | ESSI4.11

Multisource data analysis at the catchment scale to quantify and map sustainable agricultural management practices 

Maria S. Vesterdal, Tommy Dalgaard, and René Gislum

Natural environments face substantial challenges from human activities related to food, feed, and energy production. Unsustainable nutrient management is a key issue, with excess nutrients leaching into the groundwater cycle or escaping intended cropland through other pollution pathways ending up in the atmosphere or in nearby coastal systems. This nutrient loss depletes soil health, contributes to the climate crisis and impacts water quality, especially when combined with intensive farming practices lacking conservation efforts. Innovative mitigation actions, such as the Nature-based Solutions framework, designed to enhance water quality and advance sustainability in agricultural management, require thorough assessment and monitoring to encourage stakeholder participation in these strategies. Conducting research to explore the extent of their effects is thus essential, with a deeper understanding of the nutrient cycle playing a pivotal role in achieving these goals.

With the cumulatively increasing availability of remote sensing data sources and advancements in machine learning technologies, automating monitoring and assessment efforts has become a hot and important topic. The challenge is to construct transparent and transferable models capable of working with real-time data to accurately predict crop types, crop status or other desired features. The primary goal of this study is to investigate how an automated multisource data analysis approach, with a focus on remotely sensed data, can support the quantification and mapping of sustainability efforts in agricultural crop management while enhancing the understanding of nutrient flow within large-scale agricultural catchments. Centered on the Hjarbæk Fjord in Denmark, the study also aims to assess the transferability of its models across different sites in Europe. This research is part of a broader project investigating the potential of integrating permanent grasslands into crop rotations as a Nature-based Solution in the catchments surrounding Hjarbæk Fjord. The project aims to develop a decision support tool to guide the planning and optimization of grassland implementation in terms of extend and location. This tool is designed to maximize benefits across various parameters, including the number of stakeholders impacted, economic considerations, crop yield, biodiversity, and other critical factors. The output of the current study, involving the training of a deep learning model to predict cropland trends related to grassland implementation, can in turn be integrated as input for the described decision support tool.

This is an explorative study that relies on the availability of accurate ground truth data to train and validate a deep learning model, providing insights into trends associated with the implementation of sustainable management strategies. A key challenge lies in acquiring knowledge of and access to comprehensive datasets that capture relevant parameters, such as actual yield values, quantitative values of nutrients in different stages of the growth season and different nutrient pools within the cropland environment, accurate accounts of management actions and other contributors to the nutrient cycle. Additional challenges involve preprocessing satellite data to establish a robust pipeline for the automated collection of satellite imagery, ensuring a coherent time series. This includes addressing temporal and spatial data gaps through extrapolated estimations to create a consistent dataset.

How to cite: S. Vesterdal, M., Dalgaard, T., and Gislum, R.: Multisource data analysis at the catchment scale to quantify and map sustainable agricultural management practices, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6243, https://doi.org/10.5194/egusphere-egu25-6243, 2025.

EGU25-6285 | ECS | Posters on site | ESSI4.11

Can SuperDove Multispectral Satellite Data Optimize Citrus Orchard Monitoring? 

Lamia Rahali, Salvatore Pratico, and Giuseppe Modica

The increasing global demand for food and the pressing need for sustainable agricultural practices have made technological innovations essential in modern agriculture. Satellite imagery, as a cornerstone of precision agriculture (PA), provides valuable tools for monitoring crops and optimizing resource management. This study evaluates the potential of PlanetScope’s (PS) advanced 8-band multispectral sensor (SuperDove) for citrus orchard monitoring. The primary objectives are to investigate the effectiveness of PS data in assessing orchard health and dynamics and to explore its utility in detecting spatial variability within citrus orchards. The methodology involves preprocessing SuperDove data to derive key vegetation indices (VIs), such as NDVI, SAVI, and EVI, which are widely used to gain insights into the vigor and condition of citrus orchards. To assess the reliability and practicality of PS data, the study includes a comparison with free and open-source alternatives, such as Sentinel-2. This research emphasizes the importance of integrating high-resolution satellite imagery into citrus orchard management practices. While still in the early stages, the study aims to provide insights into how advanced satellite data can support sustainable agriculture.

How to cite: Rahali, L., Pratico, S., and Modica, G.: Can SuperDove Multispectral Satellite Data Optimize Citrus Orchard Monitoring?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6285, https://doi.org/10.5194/egusphere-egu25-6285, 2025.

EGU25-7430 | Orals | ESSI4.11

Improving satellite-based actual evapotranspiration estimations using data from local weather stations  

Offer Rozenstein, Jessey Kwame Dickson, and Josef Tanny

Evapotranspiration (ET) is crucial for water resource management, agricultural planning, and understanding land-atmosphere interactions. Numerous approaches are available for estimating ET at various spatial and temporal scales, including ground-based measurements, mechanistic models, and remote sensing. In this study, we aimed to enhance the accuracy and applicability of the Sentinel for Evapotranspiration (Sen-ET) plugin for estimating ET in diverse field crops in Israel. The primary objectives were to validate the Sen-ET method using eddy covariance (EC) measurements across various seasons and crop types, improve Sen-ET estimates by incorporating local weather station data, and illustrate the influence of weather station distance from measurement sites on Sen-ET accuracy.

The research was conducted across eight test sites in Israel, including fields with spring wheat, potato, cotton, and tomato. In applying Sen-ET model, we utilized high-resolution Sentinel-2 and Sentinel-3 imagery, along with ERA-5 meteorological data and local weather station inputs. The ET estimations by Sen-ET involved preprocessing satellite data, resampling meteorological data, and using a Two Source Energy Balance model to derive daily ET values. These estimates were compared against EC measurements.

The results demonstrated that incorporating local weather station data significantly improved the accuracy of the Sen-ET estimates, with most sites showing a substantial reduction in root mean square error (RMSE) of daily ET compared to the standard Sen-ET method. For example, at one of the wheat sites, the RMSE was reduced from 0.60 mm to 0.14 mm day-1. On the other hand, one of the tomato sites showed a slight deterioration, with an increase of 0.01 mm day-1 in RMSE when data from a weather station 7 km away was used. However, when a closer weather station at 1.17 km was used, the RMSE was reduced by 0.34 mm day-1, thus demonstrating the importance of employing representative weather data in the model.

This study underscores the contribution of localized meteorological data in refining satellite-based ET models and provides a robust approach for precise ET estimation in agricultural landscapes. The findings have significant implications for improving water resource management and irrigation practices.

How to cite: Rozenstein, O., Kwame Dickson, J., and Tanny, J.: Improving satellite-based actual evapotranspiration estimations using data from local weather stations , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7430, https://doi.org/10.5194/egusphere-egu25-7430, 2025.

Abstract: The universal contamination of arable land with potentially toxic elements (PTEs) poses a severe threat to food security and jeopardizes worldwide efforts to meet the United Nations Sustainable Development Goals (SDGs). How to obtain information on PTEs in regional agricultural soils more reliably is a priority problem to be solved. Multispectral satellite remote sensing, with its advantages of high spatial and temporal resolution, broad coverage, and low cost, offers the potential to acquire distribution information of PTEs over large areas. However, owing to the complexity of soil environments and the insufficiency of spectral information, the mechanism for retrieving concentrations of soil PTEs via multispectral satellites is not yet clear, and the accuracy needs to be improved. In this study, we aimed to assess whether employing a fusion of spectral information and environmental covariates, results in more accurate predictions of PTEs, specifically chromium (Cr) and mercury (Hg), in croplands than does employing spectral information alone. Three machine learning algorithms—kernel-based support vector machine (SVM), neural network-based back propagation neural network (BPNN), and tree-based extreme gradient boosting (XGBoost)—were developed to retrieve soil Cr and Hg concentrations. The results showed that the fusion of spectral information and environmental covariates combined with the XGBoost model performed best in retrieving both Cr and Hg concentrations with coefficient of determination (R2) values of 0.73 and 0.74, respectively. Environmental covariates are important variables for determining Cr and Hg concentrations in agricultural soils, but the ability to retrieve these element concentrations by utilizing multispectral information alone is limited. High Cr concentrations occurred in central towns and southern hilly mountains. High Hg concentrations were detected in the northwestern region and southern hilly mountains. The potential of fusing multispectral data and environmental variables to precisely retrieve soil PTE concentrations can serve as a reference for agricultural information monitoring worldwide.

Keywords: Potentially toxic elements; Sentinel-2; Environmental covariates; Machine learning; Farmland

How to cite: Zha, Y.: Retrieval of chromium and mercury concentrations in agricultural soils: Using spectral information, environmental covariates, or a fusion of both?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7525, https://doi.org/10.5194/egusphere-egu25-7525, 2025.

EGU25-7922 | Posters on site | ESSI4.11

Machine Learning-Based Rice Disease Diagnosis Through Joint Utilization of Satellite, Drone, and Weather Data 

Jae-Hyun Ryu, Kyung-Do Lee, Young-ah Jeon, Geun-Ho Kwak, Soo-Jin Lee, and Lak-Yeong Choi

Remote sensing and machine learning techniques enable precise diagnosis of crop growth anomalies, providing an effective means to mitigate production losses caused by disease outbreaks while supporting sustainable agricultural management. This study aims to detect rice diseases using satellite, drone, and weather data in a timely manner. A random forest model for rice disease detection was developed using drone imagery collected in 2023 year, where disease-damaged pixels were classified through K-means clustering, and the corresponding damaged areas were used for rice paddy disease classification model training. This model has been applied to agricultural fields in 2024 year as follows. First, Sentinel-1 and Sentinel-2 satellite data were utilized to classify paddy rice fields, with irrigated areas identified through the normalized difference vegetation index, land surface water index, and VV polarization. Second, the risk of rice disease occurrence was calculated based on air temperature, relative humidity, and precipitation. These variables represent weather conditions that can cause crop diseases. Third, drone measurements were conducted to monitor the abnormal growth of paddy rice when the risk score increased. Fourth, the location of disease outbreaks was detected using the random forest model, which uses surface reflectance at blue, green, red, red-edge, and near-infrared wavelengths as input data. Subsequently, drone spraying operations were carried out to reduce crop damage caused by the identified diseases. These results highlight the potential of agricultural management using remote sensing techniques.

Acknowledgments: This research was funded by RDA, grant number RS-2022-RD010059.

How to cite: Ryu, J.-H., Lee, K.-D., Jeon, Y., Kwak, G.-H., Lee, S.-J., and Choi, L.-Y.: Machine Learning-Based Rice Disease Diagnosis Through Joint Utilization of Satellite, Drone, and Weather Data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7922, https://doi.org/10.5194/egusphere-egu25-7922, 2025.

EGU25-7950 | ECS | Orals | ESSI4.11

Detecting irrigation amount from the integration of remote sensing data in the soil water model  

Fatemeh Khamseh and Mohammad Danesh-Yazdi

Agriculture is one of the primary consumers of freshwater globally. However, precise data on irrigation water use (IWU) at the regional scale is often lacking, which hampers the development of effective water management plans. This information gap is particularly crucial in water-stressed regions, resulting in significant resource waste. Remote sensing datasets offer a valuable opportunity to monitor irrigation patterns over extended periods at a regional scale. Since irrigation affects both soil moisture (SM) and actual evapotranspiration (ET), increases in SM and ET values following irrigation events can be leveraged to frequently retrieve IWU from remotely sensed data. In this regard, we first developed an irrigation-free soil water model in the root zone to simulate SM dynamics during non-growing periods. We then computed the residuals between the modeled SM and the 9 km root zone SM retrieved from SMAP L3, as well as the residuals between the modeled ET and both 30-m OpenET and 500-m PML, to estimate IWU. We used annual IWU data from Arizona State, USA, in 2017 to examine model performance. The simulated SM by our soil water model showed strong agreement with SMAP, evidenced by R2 = 0.68 and RMSE = 0.015 [mm3/mm3]. The estimated IWU using OpenET closely aligned with benchmark data, showing a bias of -17%. However, IWU retrieved by PML led to a much higher bias of -56%, indicating the deficiency of course-resolution ET products in capturing irrigation signals. We further found that over 97 % of the estimated IWU was attributed to ET rather than SM residuals, which is due to SMAP’s low spatial resolution, which limits its ability to resolve farm-scale irrigation volumes.

 

How to cite: Khamseh, F. and Danesh-Yazdi, M.: Detecting irrigation amount from the integration of remote sensing data in the soil water model , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7950, https://doi.org/10.5194/egusphere-egu25-7950, 2025.

EGU25-8008 | ECS | Posters on site | ESSI4.11

Modeling and managing erosion in arid ravines using high-resolution satellite imagery 

Amir Mor-Mussery, Eli Zaady, and Lior Blank

Abstract

Ravines in arid lands are affected by various soil erosion processes caused by inconsistent rainfall regimes, flooding patterns, and anthropogenic interventions. These effects are expressed in the geomorphological and vegetation patterns of the ravine's land segments. To address these changes, a study was planned with the following objectives: [1] Modeling the effects of ravine erosion processes on its land-segments vegetation using high-resolution satellite imagery; [2] Suggesting analysis schemes based on remote sensing to suit land management practices for the ravine parts.  The study site is located in Migda Ravine, Northern Negev, between Gerar and Patish ephemeral streams. Due to the loess soil and extreme arid conditions, the area suffers from soil erosion and land incision. Using imaging from PlanetScope® satellite constellation (spatial resolution: 3m pixel-1, temporal: Image per 3 days, and spectral: Red-Green-Blue-Near Infra-Red bands) between 2017 and 2024, from January to August each year, NDVI median and quartiles ranges of the ravine land segments were calculated and normalized against a stabilized reference plot. Thirteen erosion processes were defined, and classified into ravine surrounding areas, banks, and ephemeral stream water flow. The findings indicate erosional processes that dramatically decreased the Normalized Fresh Vegetation Reflectance (NFVR)in 2019, with a lighter decrease in 2020. Some erosion processes were characterized by a subsequent NFVR increase after the soil erosion event, while others, such as subsurface erosion, showed a continuous NFVR decrease. Stream plots were characterized by soil deposition, which resulted in vegetation flocculation. Using vegetation change patterns, NDVI normalization, and multi-year temporal analysis can aid in formulating land management practices for the ravine land segments and predicting long-term erosional patterns.

How to cite: Mor-Mussery, A., Zaady, E., and Blank, L.: Modeling and managing erosion in arid ravines using high-resolution satellite imagery, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8008, https://doi.org/10.5194/egusphere-egu25-8008, 2025.

EGU25-8077 | Posters on site | ESSI4.11

Development of Cropping Pattern Product Using Sentinel-2 Satellite Data 

Lak-Yeong Choi, Jae-Hyun Ryu, Ho-Yong Ahn, Soo-Jin Lee, Geun-Ho Kwak, Young-Ah Jeon, and Kyung-Do Lee

Understanding cropland utilization is essential for improving agricultural productivity and efficiently managing cropland resources. Analyzing region-specific cropping systems enables the establishment of sustainable agricultural policies tailored to environmental conditions. However, conducting field surveys over extensive agricultural areas presents significant challenges. Satellite data for agricultural monitoring provides continuous and large-scale information for cropland. The purpose of this study is to develop a cropping pattern product for annual crops using satellite data. The study area is ‘Gimje-si’ in the Republic of Korea. Sentinel-2 Level-2 data was acquired from 2022 to 2024. The normalized difference vegetation index (NDVI) was calculated after eliminating cloud and contaminated pixels, and then the monthly mean NDVI was computed. Cropland was extracted using a farmland boundary map in vector file format. Types of cropping patterns were classified into single and sequential (e.g., double, triple) cropping, and non-cultivated land, based on the number of peaks in the time-series NDVI data. The threshold for NDVI peaks was set to 0.4, and the minimum distance between NDVI peaks was set to 3. The final product was generated in vector format and includes monthly NDVI values, cropping patterns, and peak month information for each field. The annual map for 3 years showed changes in cropping patterns. These products were useful for detecting changes in cropland and confirming whether it was being cultivated. There was an increasing trend in the number of fields with sequential cropping from 2022 to 2024. Our results help comprehend the use and change of cropland spatiotemporally.

Acknowledgments: This research was funded by RDA, grant number PJ01676802.

How to cite: Choi, L.-Y., Ryu, J.-H., Ahn, H.-Y., Lee, S.-J., Kwak, G.-H., Jeon, Y.-A., and Lee, K.-D.: Development of Cropping Pattern Product Using Sentinel-2 Satellite Data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8077, https://doi.org/10.5194/egusphere-egu25-8077, 2025.

Accurate cultivated land parcels (CLPs) information is essential for precision agriculture. Deep learning methods have shown great potential in CLPs delineation but face challenges in detection accuracy, generalization capability, and parcel optimization quality. This study addresses these challenges by developing a high-generalization multi-task detection network coupled with a specialized parcel optimization step. Our detection network integrates boundary and region tasks and design distinct decoders for each task, employing performance-enhancing modules as well as more balanced training strategies to achieve both accurate semantic recognition and fine-grained boundary depiction. To improve network's ability to train more generalized models, our study identifies the variations in image hue, landscape surroundings, and boundary granularity as the key factors contributing to generalization degradation and employ color space augmentation and attention mechanisms on spatial and hierarchy to enhance the generalization. Additionally, the parcel optimization step repairs long-distance boundary breaks and performs object-level fusion of delineated regions and boundaries, resulting in more independent and regular CLP results. Our method was trained and validated on GaoFen-1 images from four diverse regions in China, demonstrating high delineation accuracy. It also maintained stable spatiotemporal generalization across different times and regions. Comprehensive ablation and comparative experiments confirmed the rationale behind our model improvements and demonstrated our method's effectiveness over existing single-task models (SegNet, MPSPNet, DeeplabV3+, U-Net, ResU-Net, R2U-Net), and recent multi-task models (ResUNet-a, BSiNet, SEANet). 

How to cite: Zhu, Y. and Pan, Y.: A deep learning method for cultivated land parcels (CLPs) delineation from high-resolution remote sensing images with high-generalization capability, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8391, https://doi.org/10.5194/egusphere-egu25-8391, 2025.

EGU25-8765 | ECS | Orals | ESSI4.11

Using Remote Sensing Spectral Image Dynamics for early prediction of biotic stress in wheat: lessons from Armenia and southern Russia 

Igor Sereda, Andrey Medvedev, Grigor Ayvazyan, and Shushanik Asmaryan

Winter and spring wheat are among key agricultural crops in the Republic of Armenia, and represent a significant share of grain production. However, their yield is threatened to substantially decline due to the negative impact of various biotic factors, including weeds and phytopathogens such as rust, powdery mildew, and tan spot. Remote sensing methods, particularly multitemporal dynamics of plant spectral imagery, offer opportunities for early detection and monitoring of these diseases. Early identification allows for timely management interventions to stabilize crop conditions, preserve yields, and enable mapping of problem areas before scheduled applications, allowing more effectively application of herbicides and fungicides.

Hyperspectral spectrometry of winter wheat crops under increased pathogen stress, together with control plots without increased pathogen stress, were studied in experimental fields in southern Russia (Krasnodar Krai) between 2017-2023. The results show that the temporal dynamics in reflectance during the spring-summer growth period of winter wheat likely indicate disease levels, where the period between stem elongation and heading was identified as crucial. A series of high-frequency spectral measurements (every 2–3 days) allowed the classification of areas with infected and healthy plants (accuracy of 70–88%) but also reasonably accurate predictions of the maximum development stage of various pathogens (R² = 0.48–0.55) 10–12 days before peak development. Moreover, these patterns were confirmed using data from ground-based spectrometry, UAVs, and satellite imagery.

Additionally, this methodology was tested on spring wheat fields in the Republic of Armenia (Aragatsotn, Nerkin Sasnashen) in 2024. Using a series of multitemporal UAV surveys, the fields were divided into zones based on the temporal behavior of spectral imagery that successfully identifies zones of weed emergence and negative consequences of agronomic errors. However, identification of more sensitive spectral regions with pathogen hotspots was hindered by the high heterogeneity of the fields.

Based on these methodologies, we defined the optimal dates for initiating phytosanitary monitoring for different regions in Armenia. This part of the investigation shows that zoning territories by the timing of the phenophase "stem elongation" with an error <10 days is crucial for the start of intensive spectral monitoring, and can be achieved by combining NDVI data with meteorological and topographical parameters.

Altogether, the results demonstrate the early diagnosis of biotic stress in plants is feasible using spectral data and can improve decision-making for field treatments in the long term. The early detection of biotic stress in plants enhances the potential of precision agriculture, as time is a crucial factor in addressing these challenges. Furthermore, the described methods have shown the capability to be scaled from local experiments, as is currently the case in most studies, to a regional scale.

How to cite: Sereda, I., Medvedev, A., Ayvazyan, G., and Asmaryan, S.: Using Remote Sensing Spectral Image Dynamics for early prediction of biotic stress in wheat: lessons from Armenia and southern Russia, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8765, https://doi.org/10.5194/egusphere-egu25-8765, 2025.

EGU25-9499 | Posters on site | ESSI4.11

Spectral-based monitoring methods to optimise precision irrigation in maize 

Attila Nagy, Andrea Szabó, Gift Siphiwe Nxumalo, Erika Budayné Bódi, and János Tamás

Precision irrigation is one of the fundamental areas of modern agriculture that aims to manage water use more efficiently and sustainably. Continuous monitoring of crop status is essential for the optimisation of irrigation systems, in which spectral-based monitoring methods play a key role. These methods use the spectral properties of the light reflected or absorbed by plants to determine vegetation indices, soil moisture and other plant life parameters. Measurements in the optical and infrared (IR) wavelengths are particularly important as these wavelengths are sensitive to the biochemical and physical properties of plants, such as chlorophyll content, nitrogen levels and water content.

The primary aim of the study is to expand the area of remote sensing in agricultural monitoring using laboratory, field scale proximal sensors, field an UAV imaging by creating a new rapid non-invasive approach for predicting crop health and water demand using spectral data. The study seeks to close the gap where chlorophyll estimations are generally not plant-specific by offering an integrated and refined approach to improve reliability and accessibility in chlorophyll estimation. Besides Integrating VI and thermal imaging with UAV technology can be used in precision agriculture in a number of areas, such as crop monitoring, yield forecasting and optimisation of irrigation water allocation. Furthermore, using several VIs were found to be optimal in crop coefficient estimation, so as to more precise calculation of crop evapotranspiration The ultimate result is giving new approaches to farmers and agricultural stakeholders for more precise and dependable tools for measuring crop evapotranspiration, crop health while promoting sustainability, efficiency, and scalability in irrigation practices.

The research presented in the article was carried out within the framework of the Széchenyi Plan Plus program, with support from the RRF 2.3.1 21 2022 00008 project. This research was supported by the János Bolyai Research Scholarship of the Hungarian Academy of Sciences

 

How to cite: Nagy, A., Szabó, A., Nxumalo, G. S., Budayné Bódi, E., and Tamás, J.: Spectral-based monitoring methods to optimise precision irrigation in maize, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9499, https://doi.org/10.5194/egusphere-egu25-9499, 2025.

EGU25-9634 | ECS | Orals | ESSI4.11

Assessing generalization of deep learning models for crop classification under climatic variability in Denmark 

Muhammad Rizwan Asif, Mehdi Rafiei, Rasmus Nyholm Jørgensen, Michael Nørremark, and Nima Teimouri

This study explores the impact of climatic variability on the generalization capabilities of a deep learning model for pixel-level crop classification using multi-temporal Sentinel-1 SAR data in Denmark. With agriculture accounting for 61% of Denmark’s land area, accurate and timely crop mapping is essential for providing insights into crop distribution, offering valuable information to advisors and authorities to support large-scale agricultural management, and address challenges posed by changing climatic conditions.

Our study leverages a novel deep learning architecture that combines a 3-D U-Net with a conv-LSTM module to effectively capture both spatial and temporal dependencies in crop growth patterns. We consider 14 crop types over an eight-year period (2017–2024) and growth season (May to August), with ground truth data derived from Denmark’s Land Parcel Identification System (LPIS). Our analyses reveal that climatic variables such as precipitation, temperature, and humidity significantly influence model performance across years. Notably, extreme years like 2018 (characterized by drought and high solar radiation) and 2024 (marked by record precipitation) challenge the model’s ability to generalize effectively. By correlating inter-annual model accuracy trends with climatic data, the study demonstrates the necessity of incorporating environmental context into AI-driven agricultural monitoring systems.

We also evaluate the benefits of training the model on multi-year datasets to enhance robustness against climatic variability. Our findings reveal that leveraging temporal diversity improves model performance but highlights persistent difficulties in generalizing to outlier years with extreme climate conditions. While training on multi-year datasets helps capture a broader range of crop phenological variations, the results underscore that this approach alone is not sufficient, and underscores the importance of integrating auxiliary data, such as local climatic variables, to enable models to better adapt to evolving crop growth patterns influenced by changing environmental conditions.

This work represents one of the most comprehensive evaluations of deep learning for crop classification, spanning eight years and covering over 1.5 million hectares of agricultural land. By linking model performance to climatic variability, this study provides critical insights for improving the generalization capabilities of deep learning models in precision agriculture. These findings not only pave the way for enhanced crop monitoring under diverse climatic scenarios but also emphasize the potential of integrating climate-resilient AI technologies to address global agricultural and environmental challenges.

How to cite: Asif, M. R., Rafiei, M., Jørgensen, R. N., Nørremark, M., and Teimouri, N.: Assessing generalization of deep learning models for crop classification under climatic variability in Denmark, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9634, https://doi.org/10.5194/egusphere-egu25-9634, 2025.

EGU25-9672 | ECS | Orals | ESSI4.11

Barley Yield Estimation Using Regression Models and Spatial Pattern Analysis 

Faten Ksantini, Miguel Quemada, Andrés F. Almeida-Ñauñay, Ernesto Sanz, and Ana M. Tarquis

Precision agriculture (PA) has emerged as a key strategy for optimizing agricultural production. Using data-driven technologies such as sensors and satellite imagery, PA improves the efficiency of agricultural processes. Accurate crop yield estimation is an essential component of PA. An important aspect of yield estimation within PA is the ability to assess and map spatial variations in yield in an agricultural field. Understanding these spatial patterns enables more precise management decisions and targeted interventions.

Therefore, this study aimed to develop two regression approaches, multiple linear regression (MLR) and random forest regression (RFR), to estimate crop yield using sixteen input variables with a 6 m resolution. These variables were obtained using different sensors, reflecting the soil and crop spatial variability. The estimation performance of the studied approaches was assessed using the coefficient of determination (R²), showing very satisfactory results (R² > 0.85) for both approaches.

The spatial distribution of barley yield was assessed, focusing on identifying areas of high and low productivity within the field. RFR demonstrated its ability to capture yield patterns. By incorporating spatial factors, RFR effectively modelled the varying yield potential in the crop field.

 

Keywords—precision agriculture, multiple linear regression, random forest regression, spatial pattern, barley

 

Acknowledgments: Financed by Ministerio de Ciencia e Innovación, Spain (PID2021-124041OB-C22)

 

How to cite: Ksantini, F., Quemada, M., Almeida-Ñauñay, A. F., Sanz, E., and Tarquis, A. M.: Barley Yield Estimation Using Regression Models and Spatial Pattern Analysis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9672, https://doi.org/10.5194/egusphere-egu25-9672, 2025.

EGU25-9872 | ECS | Orals | ESSI4.11

Remote Sensing-based Wheat Area and Yield Estimation: Insights from Uttarakhand, India 

Priya Singh and Kritika Kothari

India is one of the world's leading exporters of wheat grain, making monitoring its growth and yield one of the country's top economic priorities. This study aimed to develop a methodology for delineating wheat cultivation areas and estimating wheat yields using Landsat 8 (30 m spatial resolution) data for the Nainital and Udham Singh Nagar districts of Uttarakhand, India. The cultivated wheat fields were identified using a supervised classification-based Random Forest (RF) algorithm during the growing season from November 2020 to April 2021. To characterize the wheat class, a total of 239 and 226 wheat points, along with 201 and 166 non-wheat geometry points, based on NDVI time series were allotted for Nainital and Udham Singh Nagar districts, respectively. The calculated wheat area was found to be 778.94 sq. km and 209.48 sq. km, compared to the actual reported areas by the Agriculture Department, Government of Uttarakhand of 1059.61 sq. km and 212.78 sq. km for Udham Singh Nagar and Nainital, respectively. The RF algorithm showed an underestimation for both districts, achieving a kappa coefficient of 0.97, producer accuracy of 0.97, user accuracy of 0.96, and overall accuracy of 0.98 for the Nainital district. For the Udham Singh Nagar district, the kappa coefficient was 0.89, with producer accuracy of 0.89, user accuracy of 0.93, and overall accuracy of 0.93. The study also utilized weather data along with Landsat 8 imagery as inputs for the Carnegie-Ames-Stanford Approach (CASA) to estimate wheat yields and get spatial wheat yield maps. The estimated mean yields were 3.73 t ha⁻¹ and 3.37 t ha⁻¹, whereas the actual mean yields were 3.82 t ha⁻¹ and 4.45 t ha⁻¹ for Nainital and Udham Singh Nagar districts, respectively. The study demonstrates the potential of combining remote sensing and supervised classification techniques for reliable wheat yield estimation in data-scarce regions, which can be a promising tool for agricultural policy and decision-making.

Keywords: Crop classification, Landsat 8, random forest, wheat, spatial yield map 

How to cite: Singh, P. and Kothari, K.: Remote Sensing-based Wheat Area and Yield Estimation: Insights from Uttarakhand, India, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9872, https://doi.org/10.5194/egusphere-egu25-9872, 2025.

EGU25-10478 | ECS | Posters on site | ESSI4.11

Correlation between NDVI and soil sensor data collected by UAV 

Andrea Szabó, Erika Budayné Bódi, Ademola Blessing Blessing, Sándor Kun, Éva Nikolett Kiss, János Tamás, and Attila Nagy

The development of UAVs and the reduction in the weight of payload-bearing devices is making remote sensing of crops possible. This technology is cheaper, more time-efficient and produces higher resolution images in a non-destructive way. Another important feature of drone imagery is its ability to monitor crops on a regular basis. The raw data collected by drones can be integrated into models for analysis and further corrective measures can be created to improve crop yields. Drones are capable of assessing soil conditions, assisting in irrigation, fertilizer application and monitoring crop health. The Normalized Difference Vegetation Index (NDVI) was used to quantify the greenness of vegetation to assess changes in vegetation density and health. When near-infrared light reaches the leaves of a healthy plant it is reflected back into the atmosphere, as the amount of chlorophyll produced by the plant decreases, less near-infrared radiation is reflected back. The result can then be used to assess the overall health of the plant. The values are calculated for each pixel of your map, giving you an index in the range -1 to 1.

 

4 sampling points (A-D) were selected in the sample area Nyírbator, Hungary. Soil moisture and soil temperature probes were deployed at three depths in the points and data were downloaded during bi-weekly sampling and measurements. The vegetation monitoring of the irrigated and non-irrigated area was carried out by taking NDVI images every 2 weeks using UAV remote sensing. During the NDVI processing of the irrigated area, only the first half of the area was captured for the initial images, at the beginning of the vegetation. NDVI images were processed in Pix4D and ArcGIS Pro software. In ArcGIS Pro, the minimum, maximum, mean and standard deviation values for the study area were observed and subsequently evaluated separately point by point using a zonal statistics algorithm.

 

In the study area, a larger temperature variation is observed for the deployed soil probes at a depth of 10 cm, which underlines the sensitivity of the surface temperature to environmental conditions. With increasing depth, a gradual decrease in temperature is observed, indicating the influence of soil properties on heat retention and dissipation. Consistently fluctuating moisture levels near the surface (at a depth of 10 cm) were observed in response to precipitation or irrigation events. The fluctuation of the curves gradually decreases with increasing depth. At all depth levels, a more consistent linear gradient is observed, reflecting the prolonged drought conditions in the soil. This observation is consistent with the low mean NDVI values observed simultaneously in the same zone. The data show that the irrigated area tends to have higher average NDVI values than the non-irrigated area, which has significantly lower values.

 

 

 

 

This research was supported by the János Bolyai Research Scholarship of the Hungarian Academy of Sciences. The research presented in the article was carried out within the framework of the Széchenyi Plan Plus program with the support of the RRF 2.3.1 21 2022 00008 project.

How to cite: Szabó, A., Budayné Bódi, E., Blessing, A. B., Kun, S., Kiss, É. N., Tamás, J., and Nagy, A.: Correlation between NDVI and soil sensor data collected by UAV, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10478, https://doi.org/10.5194/egusphere-egu25-10478, 2025.

EGU25-11964 | Orals | ESSI4.11

What influences alpine pasture productivity? Exploring the relation among topography, climate, and biomass using remote sensing. 

Fabio Oriani, Helge Aasen, Manuel Schneider, and Pierluigi Calanca

Mountain pastures are a biodiversity rich and heterogeneous ecosystem of the Alps influenced by a complex topography and a variable climate. Understanding the impact of these factors on pasture productivity is of primary importance for forage production and ecosystem preservation.

We present here a regional analysis covering the alpine pastures in the Grisons Canton (eastern Switzerland, 1997 sq. km), for which we developed a collection of high-resolution (10-m) annual growth indicators based on the Enhanced Vegetation Index (EVI) derived from Sentinel-2 images, from 2016 to 2024. We correlate our growth maps to a 1-km gridded climate dataset (Meteoswiss) and a 10-m digital elevation model (Swisstopo) to understand which weather factors - rainfall, temperature, or radiation - influence the most the growing season and from which period of the year. In addition, we explore the variability of these dependencies in space, in relation to elevation and derived topographic descriptors, e.g. slope or valley orientation.

This analysis shades light on the climate dynamics impacting the most the growing season in conjunction to a complex local topography. The results can be used to identify vulnerability levels along the elevation profile, influenced by soil depth and valley orientation, where growth varies the most from year to year in function of annual weather variations. In these zones, pasture management will need extra flexibility measures and real-time monitoring to adapt to annual fluctuations of a future climate change.

How to cite: Oriani, F., Aasen, H., Schneider, M., and Calanca, P.: What influences alpine pasture productivity? Exploring the relation among topography, climate, and biomass using remote sensing., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11964, https://doi.org/10.5194/egusphere-egu25-11964, 2025.

Understanding and monitoring crop growth is crucial for addressing global food security challenges and promoting sustainable agricultural practices. Traditional methods of observing crop traits in plot experiments are labor-intensive, limiting their spatial and temporal resolution. While conventional satellite platforms like Sentinel-2 and Landsat have proven valuable for large-scale agricultural monitoring, their spatial resolutions and temporal gaps are insufficient for time series of small experimental plots. Recent advancements, such as PlanetLabs’ SuperDove constellation, provide an alternative by offering daily imagery at a 3 m resolution, making them suitable for small-scale plot-level analysis. Despite their high spatial detail, these images face challenges related to radiometric stability, spatial co-registration accuracy, and quality masks, which must be resolved for effective small-scale monitoring. Addressing these limitations, this research investigates the use of PlanetScope data to estimate canopy cover (CC) and leaf area index (LAI) in plot experiments. High-resolution Unmanned Aerial System (UAS) RGB imagery was used as a reference to estimate early-stage CC. By applying a machine learning-based segmentation technique, we distinguished foliage from background pixels. This segmentation enabled us to integrate UAS-derived CC estimates with 8-band multispectral imagery from PlanetLabs’ SuperDove constellation. After improving the radiometric stability and spatial accuracy of the satellite imagery, we used the multispectral data along with UAS-derived canopy cover estimates as inputs to identify the most sensitive satellite-derived vegetation indices (VIs) for estimating CC during the early growth stages. In conjunction with LAI, we generated model-based time-series growth curves covering all phenological stages. The method was validated on experimental plots in northern Switzerland, with varying soil compaction and fertilization treatments. The study demonstrates successful segmentation of high-resolution UAS-based RGB imagery, providing a robust baseline for validating satellite-derived data and training novel retrieval methods for canopy cover. Comparative analyses identify vegetation indices from PlanetScope imagery that correlate with early crop growth. This research highlights the potential of high-resolution satellite data for generating time-series growth curves, offering a valuable tool for improving crop management and optimizing resource use across diverse farming systems.

How to cite: Boos, T. and Aasen, H.: Using High-Resolution Satellite Data to Estimate Canopy Cover and Leaf Area Index in Plot Experiments, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12456, https://doi.org/10.5194/egusphere-egu25-12456, 2025.

EGU25-12606 | ECS | Orals | ESSI4.11

Comparison of zonation approaches by means of remote sensing vegetation indices for agricultural applications  

Gunay Hasanli, Sadra Emamalizadeh, Riccardo Mazzoleni, and Gabriele Baroni

Remote sensing vegetation indices play a vital role in agricultural zoning by providing detailed insights into crop health, productivity, and environmental conditions. They enable researchers and professionals to monitor environmental changes, urban expansion, and natural events with exceptional accuracy and precision. This progress has been fueled by major technological developments in satellite sensors, data processing algorithms, and analytical methods, enabling the capture of more detailed information and increased observation frequency across expansive regions. Despite these excellent opportunities, numerous image processing techniques have been suggested, each customized for particular applications, datasets, and user needs, yet no widely recognized standard methods have been established. This absence of standardization creates difficulties of interoperability, reproducibility, and consistency in analytical results. Researchers and practitioners frequently encounter challenges choosing the most suitable methods, since the effectiveness of these techniques can fluctuate based on factors like spatial resolution, temporal frequency, and the type of landscape under examination. As a result, there is an increasing demand for the creation of thorough guidelines and uniform procedures that can facilitate the use of remote sensing instruments while ensuring dependable and comparable outcomes across various studies and fields. In this research, we analyze zonation outcomes obtained from remote sensing images captured at different times, using several vegetation indices and applying various clustering techniques. The objective is to evaluate how time-related changes, the selection of vegetation indices, and the use of different clustering methods affect the precision and dependability of land classification. Through the examination of these combination performance, this comparative examination underscores both the advantages and drawbacks of each approach while offering important insights for improving classification methods in varied and changing environments.

How to cite: Hasanli, G., Emamalizadeh, S., Mazzoleni, R., and Baroni, G.: Comparison of zonation approaches by means of remote sensing vegetation indices for agricultural applications , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12606, https://doi.org/10.5194/egusphere-egu25-12606, 2025.

EGU25-13239 | Posters on site | ESSI4.11

LED-induced chlorophyll fluorescence during heat and drought stress as assessed in a microcosm experiment on sunflower 

Szilvia Fóti, Ádám Mészáros, Islam Guettala, Evelin Péli, Krisztina Pintér, Zoltán Nagy, and János Balogh

Like sun-induced fluorescence (SIF), LED-induced fluorescence (LEDIF) became frequently used to establish and analyze leaf- and canopy-level stress responses. Different plant phenotypes (trees, understory shrubs, crops, vineyards, etc.) were subjected to, in most of the studies, blue LED illumination during the night or in darkened boxes for assessing either the entire broad-band (650-850 nm) spectrum of LEDIF or one of the wavelength bands of the red (~ 690 nm) and far-red (~ 740 nm) peak emissions. It seems to be however less common to apply close to “white” LED lighting, mixed from different wavelength ranges all below 650 nm (to overcome spectral overlap of red excitation and emission) as a light source. Moreover, stress manipulation in microcosm experiments is also scarce within studies while detecting LEDIF signal changes.

In our study, we established a microcosm experiment with four treatments on sunflowers: well-watered – no heat stressed, well-watered – heat stressed, water-stressed – no heat stressed, and water-stressed - heat stressed. The plants were gradually exposed to the treatments during the two months of the experiment between October and December 2024. We captured reflectance and the broad-band fluorescence spectra above the canopy with a VIS-NIR spectrometer facing downwards toward the canopy between the LED panels. We followed the response of the plants to the imposed stress by weekly/bi-weekly measurements and analyzed the changes in the shapes of the curves. We also captured the canopy architecture with side-view photos and leaf area growth with top-view photos. There was a clear increase in the LEDIF signal during the canopy development, and then a heterogeneous response depending on the treatment.

How to cite: Fóti, S., Mészáros, Á., Guettala, I., Péli, E., Pintér, K., Nagy, Z., and Balogh, J.: LED-induced chlorophyll fluorescence during heat and drought stress as assessed in a microcosm experiment on sunflower, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13239, https://doi.org/10.5194/egusphere-egu25-13239, 2025.

Accurate and timely seasonal yield predictions before harvest are becoming ever more relevant due to increasing pressure on the agricultural sector under climate change. Especially for agricultural planning, logistics, and food markets, seasonal predictions are of significant importance in the context of food security and price stability.

A novel approach to enhance early-season yield forecasts at the regional scale will be presented. Earth observation (EO) data from the Copernicus Sentinel-3 satellite are able to trace spatio-temporal vegetation dynamics (e.g., crop phenological status, crop growth, photosynthesis via FAPAR, or chlorophyll indices) in near real-time. By deriving daily satellite composites and combining these data with physical modelling using the Lund-Potsdam-Jena managed Land (LPJmL) dynamic global vegetation model (DGVM) in a newly developed assimilation process, enhanced yield forecasts can be achieved. There are currently no interfaces for continuous assimilation of EO data for the LPJmL model, thus, approaches such as parameter forcing and ensemble methods allowing for continuous parameter optimization during the course of the growing season are presented and compared conceptually to improve the LPJmL model for seasonal yield predictions. Existing methods for model parameter calibration and optimization with EO data using machine learning are applied to agricultural areas in the study area.

While these results focus on the study area of Bavaria, southern Germany, the approach is scalable also on national or European scale. For demonstration purposes, the year 2018 – a comparably dry year – was chosen due to the availability of detailed land use data. LPJmL was designed for global simulations, hence, a regional downscaling is necessary for its application at the regional scale.

Integrating different remote sensing data sources enables a more detailed picture of plant growth, which will allow a regional early warning system for food security and farmer’s turnover in the future. The combination of process- and data-based approaches is likely to improve accuracy and lag time.

How to cite: Jörges, C., Hank, T., and Fader, M.: Chances and Challenges of Data Assimilation for Seasonal Yield Predictions Using Sentinel-3 Satellite Data and the Agro-Ecosystem Model LPJmL, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13318, https://doi.org/10.5194/egusphere-egu25-13318, 2025.

EGU25-14174 | Posters on site | ESSI4.11

Mapping Soil Organic Carbon Dynamics in Taiwan’s Agricultural Land Using Field and Remote Sensing Data. 

Miguel Conrado Valdez Vasquez, Chi-Farn Chen, Jien-Hui Syu, and Liang-Chien Chen

Soil organic carbon (SOC) stocks represent the second-largest natural carbon reservoir globally, surpassed only by the oceans. SOC plays a vital role in maintaining ecosystem health, offering numerous benefits such as enhancing soil structure, increasing nutrient availability, and boosting water retention capacity. Beyond its ecological significance, SOC is integral to climate change mitigation, given its ability to sequester atmospheric carbon dioxide effectively. Additionally, SOC contributes to improving the physical, chemical, and biological properties of soil, making it indispensable for sustainable land management. Taiwan, an island in the western Pacific Ocean, spans an area of approximately 35,800 square kilometers. Shaped like a tobacco leaf, the island extends 400 kilometers in length and 150 kilometers at its widest point. Taiwan’s landscape is characterized by a Central Mountain Range running north to south, steep slopes, and geologically fragile formations. In recent decades, Taiwan has experienced significant changes in land use and land cover, particularly in urban areas where cropland and forest land on city outskirts have been replaced by infrastructure development. These transformations have directly impacted SOC levels across the island, underscoring the need for accurate mapping to estimate SOC stocks and assess soil functionality, particularly in agricultural regions. Traditional ground sampling methods for estimating SOC, though precise, are often costly and labor-intensive. To address these limitations, alternative approaches, such as remote sensing, offer cost-effective solutions. Among various predictive modeling techniques, machine learning algorithms like Random Forest (RF) have emerged as highly effective tools for SOC estimation. RF models excel due to their ability to minimize correlation among individual decision trees and provide reliable error estimates, ensuring robust predictions.

In this study, we combined field sampling data (2010–2021) with remote sensing, topographic, and climatic datasets to estimate SOC stocks in the topsoil layer (0–30 cm) of Taiwan’s agricultural areas. Using the RF algorithm, we initially employed 23 explanatory variables and subsequently refined the model by eliminating less significant predictors, reducing the final set to 12 variables. The refined model demonstrated strong predictive accuracy, with R² values exceeding 0.70 for agriculture land in Taiwan. Our findings revealed spatial variations in SOC levels, with mountainous regions exhibiting higher SOC stocks compared to suburban and low-lying agricultural areas, where values were notably lower. SOC levels for agricultural lands ranged from a maximum of 7.14 kg/m² to a minimum of 2.55 kg/m², with an average value of 3.43 kg/m². Agricultural practices incorporating agroforestry techniques showed relatively higher SOC stocks, emphasizing the role of sustainable practices in enhancing soil carbon storage. The results of this study hold significant implications for long-term monitoring of SOC in Taiwan and provide a crucial reference for policymakers aiming to develop effective carbon sequestration strategies. By integrating field data with advanced modeling and remote sensing technologies, this research contributes to a deeper understanding of SOC dynamics and supports efforts to promote sustainable land management and climate resilience.

How to cite: Valdez Vasquez, M. C., Chen, C.-F., Syu, J.-H., and Chen, L.-C.: Mapping Soil Organic Carbon Dynamics in Taiwan’s Agricultural Land Using Field and Remote Sensing Data., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14174, https://doi.org/10.5194/egusphere-egu25-14174, 2025.

Air pollution, particularly surface ozone, has become a significant threat to agriculture in China, severely impacting the productivity of essential staple crops like winter wheat. However, the spatiotemporal variability of ozone concentrations and its interactions with other environmental factors—such as temperature and droughts—remain inadequately understood regarding their impact on agricultural productivity. To address this gap in knowledge, this study integrates multi-source remote sensing data with advanced statistical analysis and machine learning techniques to quantitatively examine the spatiotemporal variation of ozone pollution and its interactions with climate change and other environmental factors on winter wheat productivity.

The study first employs the Geographically and Temporally Weighted Regression (GTWR) model, utilizing high-resolution remote sensing data from 2013 to 2019, to assess the spatiotemporal response of winter wheat productivity to ozone pollution. To further investigate the interactions between ozone and other environmental factors, an interpretable machine learning framework is applied, specifically using the eXtreme Gradient Boosting (XGBoost) algorithm augmented by SHapley Additive exPlanations (SHAP). Additionally, a structural equation model is developed to elucidate the underlying mechanisms of these interactions. The results indicate that the negative impact of surface ozone on winter wheat has intensified annually, with significant spatial variation. Particularly in high-pollution areas, such as eastern Henan and northern Anhui provinces, the effects of ozone on winter wheat are most pronounced. Furthermore, the study reveals that the impact of ozone on winter wheat productivity varies across different growth stages, with the most severe effects observed during the later stages in May. Additionally, the research reveals the complex interactions between ozone and other environmental factors, such as temperature and aerosol concentration. Notably, the harmful effects of ozone are exacerbated under conditions of high aerosol concentration and elevated temperatures. Interestingly, drought conditions were found to partially mitigate the negative impact of ozone on productivity.

This study provides a systematic and actionable analytical framework for quantitatively evaluating the effects of ozone pollution and its interactions with climate change and other environmental factors on crop productivity. The findings underscore the need for targeted agricultural measures and pollution control strategies, particularly in high-pollution regions and during critical growth stages. These results provide theoretical support for sustainable agricultural development and climate adaptation management. Furthermore, the study contributes valuable insights into the application of remote sensing technology for large-scale agricultural monitoring, thereby enhancing the management efficiency and adaptive capacity of agricultural ecosystems in response to environmental challenges.

How to cite: Du, C.: Evaluating Air Pollution Impacts on Agricultural Productivity in China: Insights from Remote Sensing Data and Geospatial Modeling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14198, https://doi.org/10.5194/egusphere-egu25-14198, 2025.

EGU25-14688 | Posters on site | ESSI4.11

Monitoring Methane Emissions from Rice Paddies in Middle Taiwan Using Remote Sensing Data. 

Cheng-Ru Chen, Chi-Farn Chen, Nguyen-Thanh Son, Liang-Chien Chen, Tsang-Sen Liu, and Yao-Cheng Kuo

Methane (CH₄) emissions from paddy rice fields significantly contribute to greenhouse gas emissions and global climate change. In Taiwan, rice cultivation occupies approximately 20% of agricultural land. This study utilizes Sentinel-2 and Sentinel-5P satellite data to monitor methane emissions from these fields. The research follows four key steps: 1) classifying rice cropping areas; 2) detecting the phenological stages of rice; 3) correlating spatial and temporal data with rice cultivation and methane emissions; and 4) validating the results with in-situ data. The preliminary findings identify methane emission hotspots during the rice-growing seasons, revealing substantial temporal variability linked to agricultural practices such as water management, organic matter application, and rice phenology. Peak emissions occur during the early to mid-growing stages. The adoption of satellite data for monitoring emissions offers a cost-effective and scalable alternative to traditional methods, which are often labor-intensive and geographically limited. The research can also enhance the sustainable agricultural management strategies for achieving local greenhouse gas reduction targets.

How to cite: Chen, C.-R., Chen, C.-F., Son, N.-T., Chen, L.-C., Liu, T.-S., and Kuo, Y.-C.: Monitoring Methane Emissions from Rice Paddies in Middle Taiwan Using Remote Sensing Data., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14688, https://doi.org/10.5194/egusphere-egu25-14688, 2025.

EGU25-14999 | Orals | ESSI4.11

Early prediction of within-field variability wheat productive potential using Sentinel2 satellite data. 

Elena Pareja-Serrano, José González-Piqueras, and André Chanzy

Assessing agricultural production in the context of climate change is a global concern. In the recent decades, variable rate technology (VRT) for agricultural machinery has made it possible to adjust fertiliser rates on-the-go, allowing the within-field crop management. In this context, in order to select the most effective management practices, it is essential to identify the driving factors that determine yield variability, mapping the spatial distribution of these driving factors and to determine the local yield variability potential.

Mapping the homogeneous within-field areas of yield potential is used to define management zones. Remote sensing data provide a practical means of delineating these zones. The crop biophysical variable, cumulative evapotranspiration (ETccum), derived from NDVI time series and climate data, was analysed to evaluate its ability to estimate yield. In the semi-arid conditions of the Spanish Central Plateau, wheat ETccum maps were correlated with yield maps by non-linear regression with an R2 of 88%. ETccum serves as an effective proxy for yield estimation and the statistical analysis to determine the level of homogeneity within the field, the driving factors that determine yield variability, and mapping the spatial distribution of these driving factors. Nevertheless, the observed saturation effect in the biophysical variable highlights limitations that require further analysis.

Additionally, during the wheat season, expected potential yields can fluctuate in response to actual weather conditions. Consequently, updating yield predictions early in the season is critical for informed irrigation and fertilisation management decisions. The ability of ETccum to forecast yields at early phenological stages, such as flag leaf and flowering—key stages for yield formation—is examined. Finally, the stability of spatial variability patterns, compared to those derived from ETccum at maturity, is analysed as an indicator of the spatial distribution of yield drivers.

Acknowledgments: this work was supported by the research project NSBOIL (Horizon, GA 101091246).

How to cite: Pareja-Serrano, E., González-Piqueras, J., and Chanzy, A.: Early prediction of within-field variability wheat productive potential using Sentinel2 satellite data., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14999, https://doi.org/10.5194/egusphere-egu25-14999, 2025.

Effectively tracking drought effects using satellite data can be conducted by combining atmospheric data with additional information of vegetation indices (VIs) from optical data. While VIs detect drought when plant damage is often irreversible, information about the plant physiological status can help detect drought effects much earlier. Remotely-sensed solar-induced chlorophyll fluorescence (SIF), emitted directly from the photosynthetic apparatus (Drusch et al., 2017), provides such information.  When abiotic stress occurs due to an increased dissipation of thermal energy through the process of non-photochemical quenching (NPQ), the fluorescence yield is decreased, which can be measured as SIF (Berger et al., 2022, Damm et al., 2018).

Top of canopy (TOC) SIF is available from Sentinel-5P’s TROPOMI sensor since 2018 (Guanter et al., 2021, Köhler et al., 2018). This data, however, is affected by incoming radiation and canopy structure. These effects need to be removed In order to calculate the fluorescence yield in form of the quantum efficiency at leaf level (ΦF), which provides the pure information on the actual physiological status of the plant. Equation (1) uses the vegetation index NIRv (NDVI*NIR (Badgley et al., 2017)) to serve as a combined proxy of the fraction of absorbed photosynthetically active radiation (fAPAR) and the fluorescence escape probability (fesc) (Dechant et al. 2020, Liu et al. 2023). Both SIF data at 743 nm and the reflectance used to calculate the NIRv come from TROPOMI, while the photosynthetically active radiation (PAR) is provided by MODIS.

ΦF = π*SIF743canopy/(NIRv*PAR) (1)

This study presents a new multi-year (2018-2023) ΦF dataset at 0.05° resolution covering Germany with daily temporal resolution. To assess ΦF’s potential as an early drought stress indicator for agricultural and forest ecosystems, it is compared to the anomaly of subsurface water storage (sss), which serves a reference parameter for plant water availability generated by combining the hydrological model PARFLOW and common land model (CLM) (Belleflamme et al., 2023). ΦF and sss anomaly data were split into periods of prolonged negative sss anomaly indicating drought events (cross-referenced as watch/warning periods using the Combined Drought Indicator (European Commission)). Cross-correlation coefficients for different time lags were calculated to compare the datasets. The data was spatially aggregated daily and temporally averaged using a two-day rolling average.

Results show that cross-correlation coefficients for ΦF and sss anomaly are highest at a 2-day lag, dropping again after 3 days, indicating that ΦF follows the negative sss anomaly trend with a 2-day delay in both agricultural and forest ecosystems. Non-normalized canopy SIF and vegetation indices (NIRv, NDVI) showed no pattern and low cross-correlation coefficients during the observed periods. Our findings prove that ΦF has the ability to detect insufficient plant water availability and thus can be used for early drought stress detection in agricultural and forest ecosystems. The comparison of the capabilities of ΦF and TOC SIF to track short-term changes in subsurface water storage illustrates that a proper downscaling and normalization of canopy SIF is essential to use SIF satellite measurements for the early detection of drought events.

How to cite: Herrera, D., Rascher, U., Belleflamme, A., and Siegmann, B.: On the Potential of a Novel Satellite-Based Time-Series of Normalized Far-Red Solar-Induced Fluorescence to Track Short-Term Changes in Subsurface Water Storage, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15038, https://doi.org/10.5194/egusphere-egu25-15038, 2025.

EGU25-15653 | ECS | Posters on site | ESSI4.11

Comparing Different Unmixing Methods for weed detection and identification 

Inbal Ronay, Ran Nisim Lati, and Fadi Kizel

Herbicides are extensively used for weed management worldwide. However, their use is a significant cause 
of environmental pollution and human health problems. Efficient Site-Specific weed management (SSWM) 
practice attempts to reduce herbicide use and its negative impacts by adjusting herbicide application based 
on weed composition and coverage. Such an application requires high-resolution data in spatial and spectral 
domains, which is not always available. Consequently, Mixed pixels are likely to exist, creating a challenge 
to generate accurate weed maps. In this regard, Spectral Mixture Analysis (SMA) can mitigate this challenge
by exploiting subpixel information. This study assesses the potential benefits of four SMA methods for 
estimating weed coverage of different botanical groups. We examined four methods- Constrained Least 
Squares Unmixing (FCLSU), Sparse Unmixing via variable Splitting and Augmented Lagrangian (SUnSAL), 
Sparse Unmixing via variable Splitting and Augmented Lagrangian and Total variation (SUnSAL-TV) and 
the Vectorized Code Projected Gradient Descent Unmixing (VPGDU). Each suggests a distinct advantage 
for spectral unmixing. We used controlled hyperspectral and multispectral field datasets to compare the four 
methods. The controlled data included weed species characterized by distinct botanical groups, while the 
field dataset included a corn field with weeds at varying densities. We assessed the performance of the 
different methods in estimating weed coverage and composition at various spatial resolutions. Our results
demonstrated the advantages of the total variation regularization of SUnSAL-TV and the superiority of the 
SAM-based method, VPGDU, over other approaches. VPGDU was the best-performing method, with MAE 
values consistently lower than 8.6% at all resolutions, underscoring the advantage of its objective function 
in unmixing weed botanical groups and the significant effect of illumination on the results. This result was 
also consistent in the field data as VPGDU yielded the lowest MAE of 11.95%,

How to cite: Ronay, I., Lati, R. N., and Kizel, F.: Comparing Different Unmixing Methods for weed detection and identification, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15653, https://doi.org/10.5194/egusphere-egu25-15653, 2025.

EGU25-15760 | ECS | Orals | ESSI4.11

Generally applicable method for unsupervised weed detection in row crops using UAV-based high-resolution RGB imagery 

Ambroos Van Poucke, Jan Verwaeren, and Wouter Maes

Advancements in sensing technology and in machine and deep learning have expanded UAV remote sensing applications in agriculture. Most of these applications rely on supervised techniques, but generalization remains a critical and underexplored challenge. Agricultural datasets often exhibit variability across fields, sensors, crops and growth stages. While models such as convolutional neural networks (CNNs) perform well when trained on millions of samples, this approach is impractical with UAV-based agricultural data. This suggests that a location-specific, unsupervised approach might be more effective.

This study proposes a generally applicable method to map weed densities in row crops using high resolution RGB UAV data. The workflow first starts with a vegetation masking based on the Excess Green index, followed by a novel row detection model that separates intra- and interrow vegetation. Pseudo-labels generated from this step are used to train the CNN segmentation model Deeplabv3.

The method was applied on 12 maize datasets collected across multiple locations in Belgium, at different growth stages, and using three different UAV cameras, leading to ranges in ground sampling distance (GSD). The model was also applied on a public sugar beet dataset, PhenoBench, covering 3 dates was used to validate the model. Model performance was evaluated against manually annotated ground truth segmentation maps from each field (n = 50).

Semantic segmentation of crops achieved consistent mean Intersection over Union (IoU) values, exceeding 0.7 (F1-score > 0.89). Weed detection performance was relatively low in very early growth stages (IoU>0.4, F1-score > 0.6) due to limited plant sizes, but improved as weeds grew, with IoU reaching 0.63 (F1-score = 0.83) in later stages. The model was equally performant on maize and on sugar beet.

Despite these early-season limitations, the lower weed detection accuracy had minimal impact on field-level weed density maps, which are primarily used for relative density comparisons to guide site-specific herbicide applications. Regression analyses of predicted crop and weed areas against ground truth annotations showed strong linear relationships. Early-season datasets exhibited slight underestimates of weed area, whereas later-season datasets demonstrated a near-perfect 1:1 relationship (R² > 0.80). GSD proved to be a reciprocal indicator of accuracy, with the highest accuracy at GSDs below 1mm/pixel. GSD above 3 mm/pixel showed a rapid decrease in accuracy.

Overall, the proposed approach effectively generates accurate field-level weed density maps, offering a robust tool for precision weed management in agriculture.

How to cite: Van Poucke, A., Verwaeren, J., and Maes, W.: Generally applicable method for unsupervised weed detection in row crops using UAV-based high-resolution RGB imagery, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15760, https://doi.org/10.5194/egusphere-egu25-15760, 2025.

EGU25-16547 | ECS | Orals | ESSI4.11

Knowledge-encoded deep fusion for yield estimation under extreme climate stress 

Xingguo Xiong, Renhai Zhong, Qiyu Tian, Ioannis Athanasiadis, and Tao Lin

Accurately modeling the impacts of climate stress on crop growth and yield is crucial for ensuring food security. Data-driven models are increasingly utilized for yield estimation because they can learn effective crop growth features from vast amounts of remote sensing and meteorological data. However, extreme climate stress conditions have few yield labels available for these models to modeling the interaction in crop responses. The response of crops to extreme climate stress often exhibits varied delays which are captured in remote sensing observations. In this study, we explicitly encode the time lag effect quantified by remote sensing and climate stress indicators into a two-stream fusion framework for estimating crop yield under extreme climate stress. Each stream employs a pyramid structure that progressively aggregates remote sensing and climate time series into feature embeddings. A time-lag-encoded cross attention mechanism fuses feature embeddings between the two streams, while phenology-sensitivity-guided linear attention is applied on top of the pyramid structures for processing ultimate time-lag encoded features. The proposed model is evaluated across nine Midwestern states within the US Corn Belt at the county level from 2006 to 2012, simulating climate stress situations with fewer samples. End-of-season results demonstrate that the knowledge-encoded two-stream model (RMSE=1.17 Mg ha-1) outperforms both the feature-stacking-based two-stream model (RMSE=1.43 Mg ha-1) and random forest (RMSE=1.68 Mg ha-1) under extreme climate stress. The improved estimation performance indicates that knowledge-encoded data fusion is more effective than merely stacking multi-source input data. In-season results reveal that our model proficiently captures extreme events and effectively predicts yield 8 weeks in advance. The time-lag knowledge could be extended to other forms of climate stress. Also, cross attention enables integration with additional data sources to enhance the interaction modeling of complex biomass accumulation and yield formation.

How to cite: Xiong, X., Zhong, R., Tian, Q., Athanasiadis, I., and Lin, T.: Knowledge-encoded deep fusion for yield estimation under extreme climate stress, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16547, https://doi.org/10.5194/egusphere-egu25-16547, 2025.

EGU25-16843 | Orals | ESSI4.11

Explainable Machine Learning for Forest Fire Detection with Remote Sensing for Effective Rescue Planning 

Octavian Dumitru, Chandrabali Karmakar, and Shivam Goyal

In the present decade, forest fires have become more common than ever [1]. Efficient strategies to cope with fire situations, and/damage assessments need efficient automatic forest fire detection model. In this research, we propose an unsupervised eXplainable machine learning model to assess the severity of forest fire with remote sensing data. The model, namely, Latent Dirichlet Allocation is a Bayesian Generative model, is capable of generating interpretable visualizations. LDA uncertainty quantifiable and explainable [2]. We do not need labelled data to train the model. Other usefulness of the model is that it is simple to combine any kind of input data (for example, UAV images, wind speed information). In the scope of this contribution, we use Sentinel-2 spectral bands to extract information to compute indices indicating severity of fire [1]. Uncertainty of each prediction of the model is computed to ascertain robustness of the model. As a use case, we have chosen the recent forest fire incident at Los Angeles, USA [6].

The methodological approach is as the following:

1) we acquire pre-fire, post-fire Seintinel-2 images, 2) compute three indices : Normalized Difference Vegetation Index (NDVI), Normalized Burn Ratio (NBR), and Burned Area Index for Sentinel (BAIS) based on state of the art literature and generate index maps, 3) compute difference between the pre-fire and post-fire index maps, 4) apply the unsupervised xAI LDA model to retrieve semantic classes in pre-fire and post-fire Sentinel-2 band images, general corresponding classification maps and plot a binary class-to-class change map,  5) Analyze the maps with visual tool to find the most affected semantic classes (e.g., dense vegetations, urban areas etc.) and produce a data-driven estimation of per-class changes due to fire [7].

In future, we plan to fuse other data sources (e.g., wind speed information [5]) to help practical applications.

Reference:  

[1] Lasaponara, A. M. Proto, A. Aromando, G. Cardettini, V. Varela and M. Danese, "On the Mapping of Burned Areas and Burn Severity Using Self Organizing Map and Sentinel-2 Data," in IEEE Geoscience and Remote Sensing Letters, vol. 17, no. 5, pp. 854-858, May 2020, doi: 10.1109/LGRS.2019.2934503.

[2] Karmakar, C. O. Dumitru, G. Schwarz and M. Datcu, "Feature-Free Explainable Data Mining in SAR Images Using Latent Dirichlet Allocation," in IEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing, vol. 14, pp. 676-689, 2021, doi: 10.1109/JSTARS.2020.3039012.

[3] California Wildfires Live Updates: 24 Dead in L.A. as Dangerous Winds Threaten Fire Growth - The New York Times

[4] Sentinel-2 mission. Available online: https://sentinel.esa.int/web/sentinel/missions/sentinel-2

[5] Global Wind Atlas. Available online: https://globalwindatlas.info/en/about/dataset

[6] ESA news based on Sentinel-2. Available online: https://www.esa.int/ESA_Multimedia/Missions/Sentinel-2/(offset)/100/(sortBy)/published/(result_type)/images

[7] Karmakar, C.O. Dumitru, N. Hughes and M. Datcu, "A Visualization Framework for Unsupervised Analysis of Latent Structures in SAR Image Time Series", IEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing, 16, pp. 5355-5373, 2023.

How to cite: Dumitru, O., Karmakar, C., and Goyal, S.: Explainable Machine Learning for Forest Fire Detection with Remote Sensing for Effective Rescue Planning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16843, https://doi.org/10.5194/egusphere-egu25-16843, 2025.

EGU25-17615 | ECS | Orals | ESSI4.11

Automated detection of tuta absoluta (Meyrik) lesions on tomato plants using artificial intelligence 

Andrés Felipe Almeida-Ñauñay, Ernesto Sanz, Juan José Martín-Sotoca, Ruben Moratiel, Esther Hernández-Montes, and Ana M. Tarquis

The invasive tomato pest Tuta absoluta (Meyrik) poses a significant threat to global agriculture, often resulting in severe yield losses if not detected and managed early. This study investigates the application of artificial intelligence (AI) to develop an automated system for detecting T. absoluta (Meyrik) lesions on tomato plants. Leveraging open-source computational tools such as Google Colab, the research aims to provide an accessible and efficient solution through computational experiments, without requiring field trials.

A curated dataset of tomato plant images is prepared for training and evaluation. The YOLO (You Only Look Once) model is utilized for its proven effectiveness in small-object detection tasks, making it an ideal choice for identifying pest lesions. Model performance is assessed using metrics such as mean Average Precision (mAP), precision, recall, and F1-score, ensuring robust and reliable results across varying conditions. Prior research has highlighted the success of similar AI-based approaches in agricultural pest detection, achieving high accuracy while supporting sustainable farming practices  

This work emphasises leveraging multi-source data and advanced modelling approaches to enhance agricultural sustainability. By integrating sensing data and AI techniques, the study supports improved Integrated Pest Management (IPM) strategies, offering a scalable and environmentally friendly solution for pest monitoring in tomato production. Furthermore, the approach demonstrates how AI-driven insights from remote sensing can contribute to the broader goals of ecosystem productivity and nature-based solutions for climate change mitigation.

Acknowledgements: The authors acknowledge the support of the Project “LIFE23-CCA-ES-LIFE ACCLIMATE: Cultivating Resilience: Climate Change Adaptation Strategies for Greenhouses to Enhance Yield and Resource Efficiency from the Programme for the Environment and Climate Action (LIFE-EU) (project number: 101157315).

How to cite: Almeida-Ñauñay, A. F., Sanz, E., Martín-Sotoca, J. J., Moratiel, R., Hernández-Montes, E., and Tarquis, A. M.: Automated detection of tuta absoluta (Meyrik) lesions on tomato plants using artificial intelligence, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17615, https://doi.org/10.5194/egusphere-egu25-17615, 2025.

EGU25-17735 | ECS | Orals | ESSI4.11

A multi-sensor remote sensing approach to monitor illegal charcoal production sites in Somalia’s forests 

Luca de Guttry, Iqro Abdi Olow, Paolo Paron, Michele Bolognesi, Ugo Leonardi, Laura Stendardi, Giovanni Argenti, Marco Moriondo, and Camilla Dibari

Illegal charcoal production, by means of indiscriminate logging activities, poses significant threats to the stability of the drylands’ ecosystem in the Somali territory. In addition, the revenues from the charcoal trade often serve further illegal activities, exacerbating the already complex socio-political context of the country. In this work, we investigated the application of freely available multi-sensor remote sensing products (Sentinel-1 and Sentinel-2) and machine learning techniques to detect the presence of charcoal production sites (i.e., kilns) over large areas. Exploiting Google Earth Engine and open-source tools, we were able to develop a binary classification of kilns’ presence-absence for the years 2019, 2020, and 2021 in a remote area (approximately 32000 km2) north-west of Mogadishu, Somalia. Concerning the workflow, we first computed median images, spanning the first three months of each year, composed of numerous optical, SAR (Synthetic Aperture Radar), and combined vegetation indices. Images were then subtracted between consecutive years and a Support Vector Classification (SVC) algorithm was trained and validated on the indices’ values extracted from those. As a reference dataset, we employed known kilns’ locations from a preceding study by FAO-SWALIM, where photointerpretation of very high resolution images was used to individuate the appearance of illegal charcoal kilns. The evaluation of the classifications showed that our approach has great capabilities for the automatic individuation and the monitoring of illegal charcoal production sites, with R2 values and accuracy metrics ranging between 0.80-0.88 for the three considered years (2019, 2020, 2021). Moreover, mappings of the predicted presence-absence of kilns (at 10 m spatial resolution) were produced starting from the trained SVC model, giving a spatial representation of the phenomenon and allowing an assessment of the most impacted areas. In conclusion, our results represent a significant advancement in monitoring illegal charcoal production activities in Somalia, offering a reliable and transferable methodology based on accessible satellite imagery and tools.

How to cite: de Guttry, L., Abdi Olow, I., Paron, P., Bolognesi, M., Leonardi, U., Stendardi, L., Argenti, G., Moriondo, M., and Dibari, C.: A multi-sensor remote sensing approach to monitor illegal charcoal production sites in Somalia’s forests, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17735, https://doi.org/10.5194/egusphere-egu25-17735, 2025.

EGU25-17743 | ECS | Orals | ESSI4.11

Remote sensing applied to phenology monitoring in vineyards: testing through field observations 

Eduardo Jiménez-Jiménez, Guillermo Muñoz-Gómez, Beatriz Lara, Federico Fernández-González, and Rosa Pérez-Badia

In this paper we study the relationship between vegetative phenology obtained from satellite-derived vegetation indices (VIs) and vegetative and floral phenology based on field observations. The work was conducted during 2023 and 2024 in vineyards belonging to the Designation of Origin Uclés, located in the west of Cuenca province (Castilla-La Mancha region, central Spain). The field work was carried out in seven plots that are frequently ploughed and lack cover crops and green covers. All plots grow under similar conditions and the maximum distance between plots is less than 2 kilometers. Phenological sampling was carried out weekly on 20 grapevines per plot, using the BBCH scale.

Different VIs (NDVI, EVI, SAVI and SAVI2) were calculated using Google Earth Engine (GEE) and Sentinel-2 data, but EVI was selected due to its greater amplitude in the index curves. The R package Phenofit was used to clean the data, curve fitting and extraction of phenology metrics. For curve fitting, the Elmore method was used, and for phenology metrics extraction, the Threshold, Inflection and Gu methods from the Phenofit package were applied. Although Inflection and Gu differ in their approach, they both divide the curve into four phenological metrics: greenup, when index starts to growth; maturity, when the index value remains stable; senescence, when it decreases; and dormancy, when it stops decreasing and remains at a low value. Threshold considers only greenup and dormancy.

The results show that greenup is associated with the inflorescence development. This phase starts in a similar day of the year (DOY) in all plots and in the two studied years. Maturity, marked by Inflection and Gu methods, occurs between flowering and fruit development stages, that is, between DOY 140–198. The senescence period is marked between fruit development and leaf discoloration (178–310 DOY), and despite its amplitude, 75% of the observations place senescence between the final stages of the fruit and leaf discoloration. Finally, dormancy occurs between leaf discoloration and the leaf fall which is correct but usually it is marked excessively late.

Phenological metrics derived from Vegetation Indices (VIs) such as greenup (potentially related to inflorescence development), senescence (potentially related to leaf discoloration), and dormancy (potentially related to leaf discoloration and fall) can be linked to the grapevine cycle on the BBCH scale. However, more studies are needed to accurately link field phenological observations with satellite-derived vegetation indices.

This work has been funded by the Junta de Comunidades de Castilla-La Mancha (JCCM) through the project SBPLY/ 21-180501-000172 and by the University of Castilla-La Mancha (UCLM) through the project 2022-GRIN-34507. EJJ thanks to the Investigo Program for a contract co-financed by the European Social Fund Plus.

How to cite: Jiménez-Jiménez, E., Muñoz-Gómez, G., Lara, B., Fernández-González, F., and Pérez-Badia, R.: Remote sensing applied to phenology monitoring in vineyards: testing through field observations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17743, https://doi.org/10.5194/egusphere-egu25-17743, 2025.

EGU25-18129 | ECS | Orals | ESSI4.11

Temporal and Spatial Analysis of Critical Field Points Using High-Resolution Soil Water Content Estimation Employing Remote Sensing and Deep-Learning 

Mehdi Rafiei, Muhammad Rizwan Asif, Michael Nørremark, and Claus Aage Grøn Sørensen

This study presents a novel deep-learning approach for estimating Soil Water Content (SWC) with high spatial resolution across multiple soil depths. Additionally, the study identifies critical field points based on their drying-out times analyzed by SWC estimations over extended periods. Understanding potential critical points regarding SWC allows operators of heavy agricultural equipment to gain insight into the field's traits and prevent excessive soil compaction. Additionally, this information can support more strategic and efficient harvesting plans by accounting for the impact of varying drying patterns on crop growth and soil strength to not only minimize soil degradation but also maximize yield production, offering a more productive and sustainable crop production.

In this regard, our proposed method offers a practical approach to integrating diverse data types, including:

  • Spatial data: remote sensing data (Synthetic Aperture Radar (SAR) and vegetation index), land elevation, and soil profiles at various depths (soil content and bulk density).
  • Temporal data: historical weather information (precipitation, temperature, wind, and global radiation).
  • Contextual data: date, groundwater level, and crop type.

Previous machine learning and numerical models primarily used temporal and contextual data alongside point-based parameter values as inputs. In contrast, we incorporated spatial information instead of point values, allowing the model to capture better the surrounding influences—such as elevation, water flow, and vegetation shadows—on SWC.

To be able to estimate the SWC using the comprehensive analysis of spatial, temporal, and relevant contextual factors, these inputs are processed by a novel multi-model deep learning framework comprising:

  • U-Net to capture spatial features and the impacts of 2D image data.
  • Temporal Convolutional Network (TCN) to extract temporal dependencies from weather data.
  • Feed-Forward Network (FFN) to model the influence of contextual inputs.

Our model is trained and validated using ground truth data from site measurements in the HOBE dataset. These measurements are conducted at 30 locations within the Skjern River Catchment in Western Denmark, with each data sample containing SWC at different depths: surface, 20cm, and 50cm. By utilizing data collected between 2014 and 2018 from point 1.09 in the HOBE dataset, we demonstrated that the proposed model achieved a mean absolute error (MAE) of 0.0207. For comparison, a numerical model (Daisy) and a machine learning approach that did not account for spatial context produced higher MAEs of 0.0382 and 0.0269, respectively.

Subsequently, the developed model is employed to estimate SWC over extended periods and identify critical points within fields. To achieve this, we collaborated with several farmers who manually classified their field maps into regular, late-drying, and critical parts. The distinction between the latter two categories is crucial, as our observations revealed that "not every wet point is a critical point." The collected temporal SWC data is analyzed with land elevation to differentiate between these two classes. This aspect of the study remains under investigation, and further research is being conducted to refine the classification process and validate its effectiveness.

How to cite: Rafiei, M., Asif, M. R., Nørremark, M., and Sørensen, C. A. G.: Temporal and Spatial Analysis of Critical Field Points Using High-Resolution Soil Water Content Estimation Employing Remote Sensing and Deep-Learning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18129, https://doi.org/10.5194/egusphere-egu25-18129, 2025.

EGU25-18174 | ECS | Orals | ESSI4.11

Innovative Approaches to Carbon Stock Assessment in Agroecosystems: The Potential of TLS 

Martina Leoni, Maria Vincenza Chiriacò, Simona Castaldi, and Riccardo Valentini

The European Union’s Carbon Removal Certification Framework (CRCF) establishes robust quality standards and transparent monitoring, reporting, and verification (MRV) systems to ensure the credibility of carbon removal initiatives. Reliable MRV systems are critical for maintaining the environmental integrity of European carbon farming efforts and building stakeholder confidence in carbon accounting and reporting. Achieving these objectives requires the integration of innovative technologies with traditional methods to enhance accuracy and scalability carbon stock estimations.

Within this framework, growing attention is being directed toward methodologies for estimating carbon stocks across various pools in agroecosystems. While soil carbon estimation methods are well-established, the estimation of above-ground biomass (AGB) in agroforestry systems remains underexplored. Significant challenges in this domain include the difficulty of conducting destructive sampling in productive agricultural systems, the lack of species-specific allometric equations for woody crops, and the variability in tree structure introduced by pruning and other anthropogenic interventions.

This study applies terrestrial laser scanning (TLS) in a plum (Prunus domestica L.) orchard to address these challenges and perform non-destructive sampling of AGB for carbon stock assessment. The research employs quantitative structure modeling (QSM) to estimate tree volume and AGB with high precision, demonstrating TLS's ability to overcome limitations associated with destructive sampling, offering a scalable and repeatable approach for accurate biomass estimation in agroforestry systems. Furthermore, the study highlights the role of agroforestry in carbon sequestration efforts.

The findings highlight TLS as a valuable tool for improving the precision and reliability of carbon accounting in agroforestry systems. Its ability to provide accurate, non-destructive AGB estimates supports the effective implementation of the CRCF and advances the EU’s climate goals. Moreover, the scalability and adaptability of TLS make it a promising addition to MRV frameworks, offering stakeholders practical solutions for enhancing carbon removal initiatives.

How to cite: Leoni, M., Chiriacò, M. V., Castaldi, S., and Valentini, R.: Innovative Approaches to Carbon Stock Assessment in Agroecosystems: The Potential of TLS, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18174, https://doi.org/10.5194/egusphere-egu25-18174, 2025.

EGU25-18417 | ECS | Orals | ESSI4.11

An Intercomparison of Two Satellite-Based Hyperspectral Imagery (PRISMA & EnMAP) for Agricultural Mapping: Potential of these sensors to produce hyperspectral time-series essential for tracking crop phenology and enhancing crop type mapping 

Mohamed Bourriz, Ahmed Laamrani, Ali El-Battay, Hicham Hajji, Nadir Elbouanani, Hamd Ait Abdelali, François Bourzeix, Abdelhakim Amazirh, and Abdelghani Chehbouni

In recent decades, space-borne hyperspectral sensors have demonstrated significant potential for agricultural monitoring by providing rich spectral information, improved feasibility, and cost-effectiveness compared to multispectral satellite imagery. In this study, we investigated the consistency of two hyperspectral satellite sensors, PRISMA and EnMAP, for agricultural mapping during the 2025 growing season in the Meknes region: one of the most fertile and productive areas for cereals and vegetables at the national level of Morocco. The primary objective was to conduct a comparative analysis of the two datasets and perform a binary classification (crop vs. no-crop) to support land use monitoring, inform decision-making, and enable advanced crop type mapping.

Our methodology included a correlation analysis of reflectance values across the visible to near-infrared (VNIR) and shortwave infrared (SWIR) ranges, as well as the evaluation of NDVI indices using two methods: band averaging and hyperspectral NDVI (hNDVI). Classification was performed using three machine learning algorithms—Support Vector Machine (SVM), Random Forest (RF), and CatBoost—based on 16 optimal hyperspectral narrow-bands (i.e., 427,  535, 567, 714, 775, 805, 839, 913, 977, 1175, 1246, 1295, 1717, 2077, 2191, 2343 nm) from PRISMA and EnMAP that best capture the variability of vegetation biophysical and biochemical characteristics.

Results demonstrated high Pearson correlation coefficients between the two sensors, with r=0.93 in the VNIR and r=0.91 in the SWIR ranges. NDVI comparison also showed strong consistency results, with correlations of r=0.84 using the hNDVI method and r=0.85 using band averaging. The utilization of optimal hyperspectral narrow-bands achieved superior classification accuracies of 99.95% with PRISMA and 99.65% with EnMAP, with SVM outperforming other algorithms, followed by RF and CatBoost. Moreover, an Explainable Artificial Intelligence (XAI) based analysis indicated that bands in the NIR and SWIR regions were the most critical features driving these high classification performances.

These findings highlight the consistency and complementarity of PRISMA and EnMAP for agricultural monitoring. They also demonstrate the potential of these sensors to produce hyperspectral time-series essential for tracking crop phenology and enhancing crop type mapping, thereby overcoming the constraints posed by limited revisit intervals in current imaging spectroscopy missions.

How to cite: Bourriz, M., Laamrani, A., El-Battay, A., Hajji, H., Elbouanani, N., Ait Abdelali, H., Bourzeix, F., Amazirh, A., and Chehbouni, A.: An Intercomparison of Two Satellite-Based Hyperspectral Imagery (PRISMA & EnMAP) for Agricultural Mapping: Potential of these sensors to produce hyperspectral time-series essential for tracking crop phenology and enhancing crop type mapping, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18417, https://doi.org/10.5194/egusphere-egu25-18417, 2025.

EGU25-18748 | ECS | Posters on site | ESSI4.11

Species Distribution Models: Application to the Identification of Populations and Potential Distribution Areas of the Forage Plant Bituminaria bituminosa 

Javier San Martin Loren, Jesús Fernandez Habas, and Pilar Fernandez Rebollo

The species Bituminaria bituminosa (L.) C.H. STIRT has been studied over the past two decades to be integrated as a forage crop in agro-silvo-pastoral systems due to its nutritional qualities and low water requirements (<200 mm). These efforts have led to the development of new varieties using genotypes from the Canary Islands. These varieties are expected to be utilized in mixed or monoculture systems, leveraging their drought tolerance to extend the availability of high-quality feed, thus reducing costs during the forage shortages of the summer season. The ability of Bituminaria to fulfill this role in Mediterranean basin farms will largely depend on its adaptation to environmental conditions.

This study aims to explore the circum-Mediterranean distribution of Bituminaria using Species Distribution Models (SDMs) and 33,132 occurrences from the GBIF platform on natural populations of the species. Bioclimatic, edaphic, geomorphological, and satellite-derived variables were used in model development through the biomod2 package in R, achieving ensemble model metrics with a mean True Skill Statistic (TSS) of 0.78. Eight clusters have been proposed to group occurrences based on the most important variables identified in the ensemble model, which also aids in identifying isolated populations or localized scenarios that may serve as a foundation for breeding programs aimed at improving specific traits. These results will contribute to a deeper understanding of the ecology, phenotypic plasticity, population dynamics, movement patterns, and evolutionary processes within the genus Bituminaria.

How to cite: San Martin Loren, J., Fernandez Habas, J., and Fernandez Rebollo, P.: Species Distribution Models: Application to the Identification of Populations and Potential Distribution Areas of the Forage Plant Bituminaria bituminosa, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18748, https://doi.org/10.5194/egusphere-egu25-18748, 2025.

Scalably sensing/estimating local information of environment, management, and crop at the field level is the first step of a System-of-Systemssolution to quantify field-level agroecosystem dynamics (Guan et al., Earth-Science Reviews, 2023). This sensing effort involves two major and inherently connected tasks: (1) ground truth collection, and (2) cross-scale sensing. Agricultural ground truth is scarce and expensive to collect, however, the need for ground truth data is non-negotiable and should be a major investment with public funding. We have developed cross-scale sensingapproaches to scale-up ground truthcollection to large scales. In this talk, we will review our recent progress in using "cross-scale sensing" to accurately estimate critical variables of agroecosystem dynamics, covering management practices (e.g. tillage practice, crop rotation, cover crop adoption, irrigation), environmental conditions (e.g. soil properties), and crop traits and conditions (e.g. LAI, Vmax, phtosynthesis, crop yield). We will also identify current challenges and future opportunities to further advance remote sensing for sustainable and precision agriculture. 

How to cite: Guan, K.: Recent progress in remote sensing for advancing sustainable and precision agriculture, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19065, https://doi.org/10.5194/egusphere-egu25-19065, 2025.

EGU25-19406 | ECS | Posters on site | ESSI4.11

Assessment of Retention Basin Potential Using Active Remote Sensing 

Dávid Pásztor, Attila Nagy, Zsolt Fehér, and János Tamás

The increasing frequency of drought periods and the intensification of precipitation distribution extremes in Central Europe, particularly in eastern Hungary, pose significant challenges for water resource management. The Great Hungarian Plain (Alföld) experiences an annual precipitation deficit of 150–250 mm, exacerbating the adverse effects of drought. The Eastern Main Canal (Keleti-főcsatorna) plays a crucial role in water supply, transporting 300–400 million m³ of water annually as part of the Civaqua program. This initiative aims to channel water from the Tisza River to the Tócó stream, ensuring sustainable water supply for the region and maintaining critical water levels in local reservoirs, including the Vezér Street Retention Basin. The basin serves not only water retention and flood control purposes but also provides recreational opportunities for the local community.
This study aims to evaluate strategies for maximizing the capacity and efficiency of retention basins by optimizing the water supply from the Tisza River and the Eastern Main Canal, particularly during drought periods. Additionally, the research explores the potential of basin retention for the storage of precipitation and excess water within the basin and surrounding landscapes. Such retention solutions contribute to efficient water resource management, mitigating drought impacts and enhancing the long-term sustainability of water management practices.
The research employed active remote sensing technologies, including the Apache 3 unmanned surface vessel equipped with a monobeam sonar, providing depth measurement accuracy within 1% of the measured depth. For terrestrial surveys, the Stonex X120GO SLAM Laser Scanner was utilized, delivering millimeter-level precision in 3D mapping. The integration of these technologies enabled the development of detailed basin models, capturing both underwater and aboveground features of the retention basin. The primary focus was the Vezér Street Retention Basin, which serves flood control, water retention, and recreational functions in the Debrecen area.
The lowest point of the Vezér Street Retention Basin is at an elevation of 110.65 m above Baltic Sea level, while the highest point of the basin crown is 114.39 m, resulting in a maximum depth of 3.74 m. The basin’s total storage capacity, when fully saturated, is 39,213.59 m³, with a water surface area of 16,354.93 m². At the average water level of 113.69 m, the basin holds approximately 28,253.2 m³ of water, with a water surface area of 15,000.08 m². During the summer, under conditions of 20°C, average atmospheric pressure, and humidity, evaporation rates reach 3 mm/day/m², resulting in a daily water loss of 45,000.24 mm/day. The aquatic biodiversity of the basin is characterized by the presence of Typha species, which serve as critical ecological indicators.
The preliminary findings highlight that active remote sensing methods, such as sonar and the Stonex X120GO SLAM Laser Scanner, provide reliable tools for maximizing basin capacity and developing efficient water retention strategies.

 

The research presented in the article was carried out within the framework of the Széchenyi Plan Plus program with the support of the RRF 2.3.1 21 2022 00008 project.

How to cite: Pásztor, D., Nagy, A., Fehér, Z., and Tamás, J.: Assessment of Retention Basin Potential Using Active Remote Sensing, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19406, https://doi.org/10.5194/egusphere-egu25-19406, 2025.

EGU25-19560 | ECS | Orals | ESSI4.11

Assessment of phenology of winter wheat using Sentinel 2 multispectral data for varying sowing dates  

Hitesh Upreti, Chinthamaneni Sriyodh, and Manoj Yadav

Wheat is one most widely grown and consumed crops globally. Region-wise, the north Indian plains are one of the largest producers of wheat in the world. However, there remains a substantial variation in the sowing dates and thus the phenology of wheat grown in the area owing to variation in cropping patterns, soil type and agricultural practices. In this study, field data including the extent of wheat crops along with their sowing and harvest dates were collected in the Gautam Buddha Nagar district of Uttar Pradesh, India during the 2022-23 crop season. The study region is then classified into croplands and further into wheat and non-wheat areas using the random forest classifier in the Google Earth Engine. On the basis of the sowing dates, the study region is divided into early sowing (sowing date before 10 November 2022) and late sowing (sowing date after 25 November 2022) areas. The phenology of the wheat agricultural fields is analyzed using the normalized difference vegetation index (NDVI) derived using the Sentinel 2 surface reflectance data product available in the Google Earth Engine. Results showed that the early sowing wheat has the largest period (6 to 7 weeks) in which canopy cover was near maximum. The same period for late sown wheat was found as 4 to 5 weeks for late sown wheat. In general, the peak vegetation density for the crop season decreased as the sowing time of the wheat was delayed. The average value of peak normalized difference red-edge index (NDRE) was found as 0.67 (in second week of February 2023) and 0.62 (in first week of March 2023) for the early and late sown wheat, respectively. The lengths of the crop seasons of the early and late sown wheat were found as 140 and 120 days, respectively. The findings of the present study can be extrapolated to understand the phenology as well as the yield patterns of the wheat in one largest wheat producing regions in the world.

How to cite: Upreti, H., Sriyodh, C., and Yadav, M.: Assessment of phenology of winter wheat using Sentinel 2 multispectral data for varying sowing dates , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19560, https://doi.org/10.5194/egusphere-egu25-19560, 2025.

EGU25-19779 | ECS | Posters on site | ESSI4.11

Integrating Orthophotos and Field Data for Precision Vineyard Yield Prediction: A Case Study of Tempranillo Grapevines 

Maite Novellón, Sara Lacalle, Ana María Tarquis, and Pilar Baeza

Anticipating the response of grapevines to environmental variability is crucial for opti-mizing field management practices. This study explores the interaction between vines and their habitat across the growing cycle to inform more effective vineyard management. The research was conducted at the "Alhambra" plot in Ciudad Real (38.8089720, -3.0705830), which spans approximately 6 hectares of irrigated Tempranillo (Vitis vinifera L.) vines. Vine spacing is 3.05x1.54 m², and the training system is a double guyot pruned, vertical shoot positioning. The study utilizes data collected over 2024.


Within the plot, three replicates of 30 plants each were sampled. Measurements were taken from consecutive rows, 15 plants each. At the phenological stage of separated clus-ters, the number of clusters was recorded, while berry weight and the number of berries per cluster were assessed at veraison and harvest. Yield partitioning was determined at harvest. Additional parameters were also measured, including total soluble solids, surface area, pruning and shoot weight.


A custom script was developed to analyze the orthophotos of the vineyard to quantify the trellis length occupied by vines, excluding gaps where vines were missing. This method enables precise calculation of the vine-covered productive area. By combining these or-thophoto analyses with field-estimated yields per linear meter of vine, the study could provide accurate vineyard yield predictions. The accuracy and effectiveness of this inte-grated methodology are thoroughly evaluated.


Acknowledgements BigPrediData

How to cite: Novellón, M., Lacalle, S., Tarquis, A. M., and Baeza, P.: Integrating Orthophotos and Field Data for Precision Vineyard Yield Prediction: A Case Study of Tempranillo Grapevines, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19779, https://doi.org/10.5194/egusphere-egu25-19779, 2025.

Andean communities in central Peru play a key role in the conservation of vicuñas (Vicugna vicugna), a protected species that depends on puna grass and flooded vegetation for food and access to water throughout the year. This study focuses on seven communities of Lucanas in Ayacucho, a dry mountainous region of Peru, emphasizing the need for accurate information to monitor resources in a context of climate change and support community decision-making. In this research, based on Google Earth Engine (GEE), we evaluated the performance of classification algorithms using Sentinel-1 (S1) and Sentinel-2 (S2) image data for rangelands classification. The process used ground-based and image-based points to train and validate the models, a filter to minimize spatial autocorrelation between training and validation sets; and spectral separability measurements using the Jeffries-Matusita (JM) distance, all of steps allowed an adequate discrimination and representation of the classes. Additionally, we used 64 feature variables (including vegetation, texture, topographic, snow, water, minerals, radar features) and applied Cloud Score+, quality assessment (QA) processor in S2 image collection, to improve classification accuracy. Random Forest (RF) algorithm achieved an overall accuracy (OA) of 92% and a Kappa coefficient of 0.908 outperforming the Support Vector Machine (SVM) algorithm, which obtained an OA of 90.9% and a Kappa coefficient of 0.895. The results show that, in the semi-captivity sectors, 1,777.5 hectares of puna grass and 319.1 hectares of flooded vegetation were identified, while in wild management areas 5,431.1 hectares of puna grass and 843.8 hectares of flooded vegetation were recorded. These findings highlight the importance of integrating remote sensing tools and machine learning algorithms to generate key information in the management of natural resources in communities.

How to cite: Ochoa, J., Juarez, H., Sotomayor, D., and De Haan, S.: Mapping Rangeland Vegetation Using Sentinel-1 and Sentinel-2 Imagery with Machine Learning: A Case Study of Vicuña Conservation in the Central Andes of Perú, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21573, https://doi.org/10.5194/egusphere-egu25-21573, 2025.

EGU25-21604 | ECS | Orals | ESSI4.11

Leaf Area Index and Leaf Chlorophyll Content estimation from hyperspectral imaging using SCOPE model inversion 

Chiara Rivosecchi, Aya Amar, Paola A. Deligios, Eline Eeckhout, Matteo Francioni, Geert Haesaert, Luigi Ledda, Adriano Mancini, and Wouter H. Maes

Leaf Area Index (LAI) and Leaf Chlorophyll Content (LCC) are key vegetation indices for modeling energy and mass exchange between the atmosphere and land surfaces and can therefore be utilized for yield prediction. Consequently, suitable methods have been developed to retrieve LAI and LCC from remotely sensed data. Among these, the inversion of Radiative Transfer Models stands out as a promising approach, as it addresses the issue of limited transferability and minimizes the need for extensive field measurements also accounting for crop variability.

The objective of this study is to assess the applicability of the Soil Canopy Observation of Photochemistry and Energy Fluxes (SCOPE) model for estimating LAI and LCC of potato (Solanum tuberosum L.) using time series of hyperspectral images captured by an uncrewed aerial vehicle. A field experiment was conducted in Belgium from June to October 2024, involving two potato varieties, early and late, subjected to two nitrogen fertilization levels and six different biostimulants. Throughout the crop growth cycle, hyperspectral UAV images were captured biweekly using the Specim AFX10 camera. On the same days, in situ measurements of LAI and LCC were performed. LAI and LCC were estimated using a look-up table (LUT) approach based on the inversion of the SCOPE model. A cost function (norm2 distance) was employed to sort the LUT and identify a set of spectra that minimized the distance between measured reflectance and simulated reflectance in the LUT. The estimated LAI and LCC values were then compared with their corresponding in situ measurements.

Preliminary results indicate that simulated LAI and LCC showed potential for use in designing models to predict measured LAI and LCC (R2=0.26 and R2=0.30, respectively, p<0.001). In conclusion, simulated LAI and LCC correlated well with measured values for the late variety at the beginning of the crop cycle. Future work will focus on extending the analysis to cover the entire season, incorporating remote sensing observations into the parametrization of a crop growth model for yield predictions.

How to cite: Rivosecchi, C., Amar, A., Deligios, P. A., Eeckhout, E., Francioni, M., Haesaert, G., Ledda, L., Mancini, A., and Maes, W. H.: Leaf Area Index and Leaf Chlorophyll Content estimation from hyperspectral imaging using SCOPE model inversion, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21604, https://doi.org/10.5194/egusphere-egu25-21604, 2025.

EGU25-21750 | ECS | Posters on site | ESSI4.11 | Highlight

PANGEOS COST action: Uncertainty propagation in remote sensing  

Egor Prikaziuk, Gary Llewellyn, Laura Mihai, Agnieszka Bialek, Andreas Hueni, Mike Werfeli, Jose Luis Gomez-Dans, Jochem Verrelst, Jose Luis Garcia-Soria, Joseph Fennell, Dessislava Ganeva, and Shawn Carlisle Kefauver

 

Pan-European Network of Green Deal Agriculture and Forestry Earth Observation Science (PANGEOS) funded by the European Cooperation in Science and Technology (COST) organisation brings together researchers to share their expertise and bring up a new generation of scientists. In October 2024 PANGEOS conducted an intensive 5-day summer school where more than 20 participants learnt how to propagate uncertainty of spectral measurements to uncertainty in higher-level products. The training material in the form of Python Jupyter notebooks is publicly available on GitHub https://github.com/pangeos-cost/uq-training.

This presentation is going to highlight the steps of uncertainty propagation from ground measurements through vegetation indices and retrieved plant traits towards higher-level model estimates, like gross primary productivity and evapotranspiration. All three pathways of retrieval uncertainty estimation, regression-based (vegetation indices), radiative transfer model-based and hybrid, are demonstrated. In addition, challenges of uncertainty propagation through satellite imagery are discussed in a separate block.

Finally, a highlight of current and future activities of the PANGEOS COST action will be given.

Acknowledgement

This abstract is supported by the EU COST (European Cooperation in Science and Technology) Action CA22136 “Pan-European Network of Green Deal Agriculture and Forestry Earth Observation Science” (PANGEOS).

How to cite: Prikaziuk, E., Llewellyn, G., Mihai, L., Bialek, A., Hueni, A., Werfeli, M., Gomez-Dans, J. L., Verrelst, J., Garcia-Soria, J. L., Fennell, J., Ganeva, D., and Kefauver, S. C.: PANGEOS COST action: Uncertainty propagation in remote sensing , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21750, https://doi.org/10.5194/egusphere-egu25-21750, 2025.

EGU25-2366 | Posters on site | ERE1.6

Electrical resistivity imaging of mangrove sediments, northern Taiwan 

Wei-Chung Han, Kun-I Lin, Liwen Chen, and Hsin-Chang Liu

Mangrove sediments are natural carbon sinks that may act as key components for climate change mitigation. To investigate the characteristics and distribution of the carbon-dense muds in the coastal mangrove areas of northern Taiwan, we applied both floating and submerged electrodes for subsurface resistivity imaging. After collecting the apparent resistivity data, we conducted 2D resistivity inversion and 3D modeling. Our results show that the muddy sediments are characterized by low resistivity and are primarily found in the top ten meters below the riverbed. On the other hand, a higher resistivity layer, probably indicating coarse-grained sediments, is situated below the muddy layer. Although the submerged electrodes generally provide the best data quality, the floating electrodes efficiently image the bottom of the muddy sediments. Therefore, we recommend that a combination of floating and submerged electrode methods for resistivity imaging should be an efficient approach to investigate mud distribution in mangrove sediments with shallow water depths.

How to cite: Han, W.-C., Lin, K.-I., Chen, L., and Liu, H.-C.: Electrical resistivity imaging of mangrove sediments, northern Taiwan, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2366, https://doi.org/10.5194/egusphere-egu25-2366, 2025.

EGU25-4496 | ECS | Posters on site | ERE1.6

Monitoring Illicit Rare Earth Mining in Myanmar via Self-Supervised Learning 

Ollie Ballinger

Heavy Rare Earth Elements (HREEs) are critical for the production of most electronic devices. Rapidly increasing demand for these minerals has led to a proliferation of highly polluting makeshift HREE extraction in Myanmar. Monitoring the spread of these mines is important for the preservation of human health and the environment. This paper utilizes a geospatial foundation model pre-trained using self-supervised learning to detect hundreds of rare earth mines using a single template example. This is achieved through the development of a novel method for embedding similarity search-- Cosine Contrast-- which leverages both positive and negative templates to yield more relevant results. 

How to cite: Ballinger, O.: Monitoring Illicit Rare Earth Mining in Myanmar via Self-Supervised Learning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4496, https://doi.org/10.5194/egusphere-egu25-4496, 2025.

EGU25-4908 | Posters on site | ERE1.6

Coalbed methane content prediction based on deep belief network 

Wenfeng Du, Suping Peng, and Xiaoqin Cui

Coalbed methane (CBM) is considered an unconventional gas resource. Accurate determination of CBM content can provide potential disaster warnings and guide exploration and development. Direct measurement and statistical analysis of CBM content are common techniques. Hoverer,direct measurement methods have high accuracy, but they are time consuming, labor intensive, and inefficient; statistical methods have a limited ability to solve complicated nonlinear problems, for example, CBM content prediction commonly used computational methods do not have high enough accuracy due to the small amount of training data and the shallow model structure. 3D seismic exploration has been widely used in CBM exploration and development due to its small grid size and high resolution. It will improve the accuracy of coalbed methane prediction to combine 3D seismic data with coalbed methane content. Machine learning techniques are a set of computational methods that can learn from data and make accurate predictions. In recent years,many applications of machine-learning techniques for CBM content prediction are found to be more reliable,however the results from traditional machine learning models have errors to some extent. A CBM content model based on Deep Belief Network (DBN) has been developed in this paper, with the input as continuous real values and the activation function as the rectified linear unit. Firstly, various seismic attributes of the target coal seam were calculated to highlight its features, then the original attribute features were preprocessed, and finally the performance of the DBN model was developed using the preprocessed features. Different from conventional DBN models, the proposed model uses continuous real values as the input and the rectified linear unit (ReLU) as the activation function. Training process includes pre training and fine-tuning. Pre training gives the model good initial parameters by training with unlabeled data, and fine-tuning uses a standard supervised method with labeled data to optimize the model. This paper successfully applied a DBN model to predict CBM content from a CBM 3D seismic  prospecting district. With more layers pre trained, the average error decreased from 3.69% to 2.16% and from 2% to 5.76% for the maximum error. Using a pre training strategy to initialize the model’s parameters can improve the accuracy of the model results. Compared with the typical multilayer perceptron(MLP)and the support vector regression(SVR)models, the DBN model has the smallest error, which means it is more accurate in predicting CBM content than the other two models.

How to cite: Du, W., Peng, S., and Cui, X.: Coalbed methane content prediction based on deep belief network, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4908, https://doi.org/10.5194/egusphere-egu25-4908, 2025.

EGU25-7010 | ECS | Posters on site | ERE1.6

Geophysical and geospatial characterization of mining heaps of the São Domingos Mine (Mértola, Portugal) 

Rui Jorge Oliveira, Bento Caldeira, José Fernando Borges, Pedro Teixeira, Gonçalo Rodrigues, Maria João Costa, Patrícia Palma, Mariana Custódio, Adriana Catarino, and Nadine Semedo

The São Domingos Mine (Mértola, Portugal) is an abandoned sulphide mine whose exploitation has had a long-term impact on its soil and water contamination problem covering an area of ​​approximately a length of 20 km and a width of 2 km. The mining heaps are spread along a watercourse that flows into the Chança River dam, which merges with the Guadiana River, both international rivers. This constitutes a serious environmental problem leading to contamination by heavy metals (HMs). Contamination assessment is a slow process that involves collecting soil samples for HMs analysis.

The study of mining heaps using geophysical and geospatial methods allows us to determine their depth and the volume of accumulated materials, as well as their characterization in relation to soils contaminated by HMs. We propose the use of electromagnetic induction, electrical resistivity tomography and GNSS methods to carry on the analysis.

This work is part of an interdisciplinary study that is being carried out within the scope of the INCOME Project (Inputs for a more sustainable region – Instruments for managing metal-contaminated areas). The aim is to combine data from Geophysics, Chemistry and Remote Sensing to create a tool, using Artificial Intelligence, that allows the calculation of contamination maps using less data than standard methodologies.

This is a sustainable management model that will increase optimization and reduce resources spent in the sampling and analysis phases. Moreover, the model aims to provide important real-time information for decision-making subjected to monitoring and managing pollution. It also has a high replication potential for other contaminated environments, such as landfills, industry or even intensive agriculture.

Funding: The work was supported by the Promove Program of the “la Caixa” Foundation, in partnership with BPI and the Foundation for Science and Technology (FCT), in the scope of the project INCOME – Inputs para uma região mais sustentável: Instrumentos para a gestão de zonas contaminadas por metais (Inputs for a more sustainable region: Instruments for managing metal-contaminated areas), PD23-00013. Acknowledgment: CREATE Project (R&D Unit ID 6107).

How to cite: Oliveira, R. J., Caldeira, B., Borges, J. F., Teixeira, P., Rodrigues, G., Costa, M. J., Palma, P., Custódio, M., Catarino, A., and Semedo, N.: Geophysical and geospatial characterization of mining heaps of the São Domingos Mine (Mértola, Portugal), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7010, https://doi.org/10.5194/egusphere-egu25-7010, 2025.

EGU25-7399 | Posters on site | ERE1.6

Modelling the fate of endocrine-disrupting chemicals during wastewater ozonation by fluorescence and artificial neural network 

Paolo Roccaro, Filippo Fazzino, Maria Rita Spadaro, Erica Gagliano, and Domenico Santoro

Many endocrine-disrupting chemicals (EDCs) are discharged into the aquatic environment mainly due to their incomplete removal during biological treatment at municipal wastewater treatment plants. For this reason, advanced oxidation processes (AOPs), using ozone with other oxidant agents, like hydrogen peroxide, are effective in removing EDCs. Furthermore, to reduce the risk of drinking water contamination by EDCs, it is necessary to ensure a real-time monitoring of wastewater treatment processes. Fluorescence spectroscopy could be used for wastewater quality monitoring to control the fate of EDCs in water systems. However, the complex physical, biological and chemical process involved in wastewater treatment process exhibit non-linear behaviors, which are difficult to describe by linear mathematical models. The artificial neural networks (ANNs) have been applied with remarkable success in several modeling studies including the highly non-linear ones.

The main objective of the present work was to use fluorescence data and ANN to monitor two EDCs, namely a pesticide (Diuron) and a pharmaceulical and corrosion inhibitor (Benzotriazole) during advanced wastewater treatments.

The data used were obtained from the pilot plant installed and operated by AquaSoil at the municipal wastewater reclamation plant of Fasano (Brindisi, Italy). The influent wastewater was obtained from tertiary treatment consisting of a coagulation stage by aluminum polychloride, sedimentation stage in lamella clarifiers and disinfection stage by sodium hypochlorite. An aliquot of the tertiary effluent was redirected to the pilot plant employing the O3/H2O2 advanced oxidation process. This process was operated in the patented technology commercialized by AquaSoil as MITO3X.

Diuron and Benzotriazole were analyzed using standard methos. Fluorescence data were collected using a Shimadzu RF-5301PC fluorescence spectrophotometer at different excitation emission wavelengths, while ANN model has been developed using Matlab software with ANN toolbox to match the measured and the predicted concentrations of EDCs.

The concentrations of Diuron and Benzotriazole were well correlated with selected fluorescence indexes. The combination of differente fluorescence peaks enhanced the determination coefficients of the single and multiple linear regressions. The developed ANN model that incorporated as input parameters the values of the fluorescence indices strongly enhanced the prediction of the fate of Diuron and Benzotriazole during AOPs. Therefore, the ANN-based model have been found to provide an efficient and robust tool in predicting the fate of EDCs removal. The comparison between ANN predicted data and experimental data shows the ability of artificial intelligence tools to predict EDCs concentrations with high accuracy and precision. Moreover, this model requires no additional information on the mechanism and the kinetics of chemical degradation of target contaminants. Since ANN have valuable advantages such as learning ability, dealing with imprecise, noisy and highly complex non-linear data, and parallel processing ability and due to the high sensitivity of fluorescence, it is expected that the developed fluorescence-ANN based model can be successfully applied for real-time control of AOPs employed for EDCs removal. This may also lead to AOPs optimization and cost savings.

How to cite: Roccaro, P., Fazzino, F., Spadaro, M. R., Gagliano, E., and Santoro, D.: Modelling the fate of endocrine-disrupting chemicals during wastewater ozonation by fluorescence and artificial neural network, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7399, https://doi.org/10.5194/egusphere-egu25-7399, 2025.

EGU25-10841 | ECS | Posters on site | ERE1.6

Soils chemical and biological characterization tools for managing metal-contaminated areas: case-study São Domingos mine (South of Portugal) 

Nadine Semedo, Mariana Custódio, Adriana Catarino, Gonçalo Rodrigues, Pedro Teixeira, Rui Jorge Oliveira, Patricia Palma, Bento Caldeira, and Maria João Costa

According to the European Union Soil Strategy for 2030, it is crucial to address contamination from mining areas, and its impact on watercourses. to achieve these goals, it is essential developing methodologies for identifying and monitoring contaminated areas, and implementing sustainable solutions for their recovery to protect soil health and ensure sustainable land use. In Portugal, soil and water contamination in former mining areas, is a significant environmental challenge, especially due to the presence of potentially toxic metals that can affect human health and ecosystems. São Domingos mine, located in the Iberian Pyrite Belt, is an open-pit mine, submerged in acidic drainage water, resulting from mining extraction activities carried out until the middle of the 20th century. In this sense, the objective of this study was to analyze the chemical and biological characterization of the soils of the São Domingos Mine, contributing to the development of an environmental management model for abandoned mining areas. To achieve this purpose, 11 topsoil (0-20cm) samples (A2 to A12) were collected in São Domingos mine, and the following parameters were analyzed: (i) chemical: pH (deionized water suspension of 1:2.5 (w/v)); electrical conductivity (EC) (deionized water suspension of 1:2 (w/v)); phosphorus (P) and potassium (K) (Egner-Riehm Method); total nitrogen (N) (Kjeldah method); organic matter (OM) (Walkley & Black method); (ii) biological(enzymatic parameters): dehydrogenase activity, acid phosphatase activity and β-glucosidase activity. The results evidenced pH ranged from 3 to 4 (very acidic). The EC, ranging from 115 to 5043 µS/cm, with most of the samples classified as non-saline. The percentage of OM was generally low (0.2 to 2.5%). Regarding macronutrients, the results were equally limiting, with the samples showing low levels of N (0.05 to 0.17%), P (1 to 6 mg P2O5 kg-1) and K (3 to 30 mg K2O kg-1). Analysis of enzyme parameters revealed low enzymatic activity frequently lower than the detection limit of the technique. An exception to β-glucosidase that generally had low values, (0.01 to 0.40 µmol PNP g-1 DM h-1), and phosphatase showing values among 0.27 to 0.96 µmol PNP g-1 DM h-1. This can be mainly related to the low values of pH, low percentage of organic matter and nutrients, and high amount of potentially toxic metals. These results will be extremely important in the development of the environmental management model proposed in INCOME project, as they provide essential information on the variability of the contamination in the mine area, essential information for validate the rest of the methodologies applied. Further, this type of model will be applicable to other regions of contamination, contributing to economic and tourist development, public health, and protection of local ecosystems, in line with the Sustainable Development Goals.

Funding: The work was supported by the Promove Program of the “La Caixa” Foundation, in partnership with BPI and the Foundation for Science and Technology (FCT), in the scope of the project INCOME - Inputs for a more sustainable region: Instruments for managing metal-contaminated areas, PD23-00013. Acknowledgment: CREATE Project (R&D Unit ID 6107).

How to cite: Semedo, N., Custódio, M., Catarino, A., Rodrigues, G., Teixeira, P., Oliveira, R. J., Palma, P., Caldeira, B., and Costa, M. J.: Soils chemical and biological characterization tools for managing metal-contaminated areas: case-study São Domingos mine (South of Portugal), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10841, https://doi.org/10.5194/egusphere-egu25-10841, 2025.

EGU25-11957 | ECS | Posters on site | ERE1.6

Preliminary Assessment of Metal Contamination in Mining Soils Using Sentinel-2 MSI: A Case Study of São Domingos Mine, Portugal 

Gonçalo Rodrigues, Pedro Teixeira, Rui Jorge Oliveira, Maria João Costa, Patrícia Palma, Bento Caldeira, Mariana Custódio, Adriana Catarino, and Nadine Semedo

The INCOME project (Instruments for Managing Areas Contaminated by Metals) proposes the development of an environmental management model for mining soils contaminated by metals. This study presents preliminary results obtained using the Multispectral Imager (MSI) aboard the European Space Agency's (ESA) Sentinel-2 satellite to identify contaminated soils in the São Domingos Mine, located in southeastern Portugal.

The MSI instrument offers significant advantages, including high spatial resolution (10, 20, or 60 m depending on the spectral band), open access for rapid image download, and frequent revisitation of the study area. The preliminary analysis focuses on identifying areas with fully exposed soil using spectral indices, which combine spectral measurements at different wavelengths to improve classification accuracy. Additionally, the Random Forest (RF) method, a widely recognised approach to general-purpose classification, was tested. Contaminated soils characteristically exhibit discrepancies in optical properties, such as distinct colouration, which can also be detected in the visible region bands of the MSI instrument. The Shortwave Infrared (SWIR) bands are particularly efficacious for identifying heavy metals.

The designated soil areas will be subject to monitoring for metal contamination utilizing the MSI instrument, with the prospective incorporation of hyperspectral data from satellites such as the Environmental Mapping and Analysis Program (EnMAP).

Funding: The work was supported by the Promove Program of the “la Caixa” Foundation, in partnership with BPI and the Foundation for Science and Technology (FCT), in the scope of the project INCOME – Inputs para uma região mais sustentável: Instrumentos para a gestão de zonas contaminadas por metais (Inputs for a more sustainable region: Instruments for managing metal-contaminated areas), PD23-00013. Acknowledgment: CREATE Project (R&D Unit ID 6107).

How to cite: Rodrigues, G., Teixeira, P., Oliveira, R. J., Costa, M. J., Palma, P., Caldeira, B., Custódio, M., Catarino, A., and Semedo, N.: Preliminary Assessment of Metal Contamination in Mining Soils Using Sentinel-2 MSI: A Case Study of São Domingos Mine, Portugal, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11957, https://doi.org/10.5194/egusphere-egu25-11957, 2025.

EGU25-14686 | ECS | Posters on site | ERE1.6

Traveltime tomography on the triangular mesh based on automatic differentiation 

Xin Chen, Tianze Zhang, Danping Cao, and Wenyuan Liao

Traveltime tomography recovers the background velocity field by minimizing the difference between observed and theoretical traveltime. Due to its computational efficiency and robustness, this method has been widely applied in studies of Earth's internal structure, oil and gas exploration, and other fields. However, most existing studies rely on regular rectangular grids for tomography, which exhibit limited adaptability when dealing with irregular topography and subsurface interfaces. The utilization of unstructured triangular meshes are more suitable for handling such complex study areas, and the development of traveltime tomography based on triangular meshes is necessary.

Compared with rectangular grids, the inversion method based on triangular meshes faces more complex gradient computation formulas, which has, to some extent, hindered the development of traveltime tomography. To address this challenge, we introduce automatic differentiation (AD) method to calculate the gradients more automatically, enabling the implementation of traveltime tomography based on triangular meshes. After building the forward computational graph, AD method can compute the gradient using the chain rule, thereby saving a lot of manpower in theoretical derivation, coding, and other processes. In this study, we used a finite difference method based on triangular meshes to solve the eikonal equation, accurately and efficiently calculating the traveltime in complex structural areas. Then, we integrate the eikonal solver into the current deep learning framework (e.g. pytorch), and update the velocity model with its built-in optimization algorithm after calculating the gradient in AD method. The process of traveltime tomography is completed on GPU, which can fully utilize the computing power of GPU and efficiently calculate inversion. Numerical tests indicate that the method can achieve promising inversion results and provide a suitable initial model for the full-waveform inversion. Our research provides a new approach for seismic inversion with unstructured grids, which is helpful for high-precision imaging of complex structural areas.

How to cite: Chen, X., Zhang, T., Cao, D., and Liao, W.: Traveltime tomography on the triangular mesh based on automatic differentiation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14686, https://doi.org/10.5194/egusphere-egu25-14686, 2025.

EGU25-15987 | Posters on site | ERE1.6

Aerogravity terrain correction method based on spherical coordinate system 

Linfei Wang, Dianjun Xue, Guanxin Wang, Deliang Teng, and Jinxin Zheng

      In recent years, due to the enhanced interference-resistance of airborne gravimeters and the advanced gravity anomaly calculation techniques, the China Geological Survey has carried out numerous airborne gravity survey missions in mid-high mountainous and deeply incised regions, including Tibet, Xinjiang, and Gansu. In practical applications, the measured free-air gravity anomalies need to have local topographic corrections and intermediate layer corrections to obtain Bouguer gravity anomalies for geological interpretation. Currently, commercial airborne gravity terrain correction software adopts the Nagy flat-topped prism method for near-field areas and the rod formula for far-field areas. This approach results in poor continuity between different terrain correction zones and fails to effectively eliminate terrain effects in deeply incised areas. This paper presents a novel method. By utilizing the coordinate surfaces in the spherical coordinate system, namely conical surfaces and semi-planes, the area is divided into rings (m rings) and blocks (n blocks), forming m×n "sectorial spherical shell blocks". A terrain correction calculation formula for these "sectorial spherical shell blocks" in the circular domain is derived, unifying the terrain correction formulas for both near and far regions. This unification allows for seamless connection among various terrain correction areas and obviates the need for intermediate layer corrections. The method has been validated by theoretical models, showing reliable accuracy in terrain correction value calculations. It has also been successfully applied in the West Kunlun airborne gravity survey. When compared with commercial software, it effectively eliminates terrain effects and achieves better terrain correction results.

How to cite: Wang, L., Xue, D., Wang, G., Teng, D., and Zheng, J.: Aerogravity terrain correction method based on spherical coordinate system, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15987, https://doi.org/10.5194/egusphere-egu25-15987, 2025.

EGU25-3961 | PICO | G2.5

A Cost-Effective Crowdsourced Q4DIM Method for Rapid PPP Implementation in Wide Areas 

Bo Wang, Shengfeng Gu, Jiaxi Zhu, and Jiayu Hu

As Global Navigation Satellite System (GNSS) positioning technology rapidly advances, Precise Point Positioning (PPP) has found widespread application in the mass market, particularly for vehicle navigation. PPP enhanced by atmospheric corrections was proven to be an effective rapid high-precision positioning method for wide-area users. The Quasi‐4‐Dimension Ionospheric Modeling (Q4DIM) is a flexible atmospheric model that enables enhanced PPP positioning from wide-area to regional applications. It divides the slant ionospheric delays (SIDs) from a station network into various clusters based on the latitude and longitude of the Ionosphere Piercing Point (IPP), satellite elevation, and satellite azimuth. These clusters are used for the correction of atmospheric errors in PPP and ionosphere monitoring. As devices capable of GNSS positioning become increasingly available in the mass market, effectively utilizing these observations could significantly reduce costs and broaden the range of rapid PPP services. In this contribution, we developed a crowdsourcing Q4DIM approach, where users upload SIDs verified for integrity to the cloud server, which classifies and stores the data based on accuracy, location, and the level of services utilized. Then, the cloud server constructs and disseminates diversity Q4DIM maps according to the different level attributes of SIDs. Finally, the users utilize the updated Q4DIM maps to achieve faster and more precise positioning. 144 sets of control experiments are conducted with observations from European Continuously Operating Reference Stations (CORS). Stations with an average inter-station distance of about 200 km are chosen as reference stations that are used for extracting the original Q4DIM map. The remaining stations are established as dynamically estimated crowdsourced stations for extracting the crowdsourced Q4DIM map. Results show that the performance of PPP enhanced by the crowdsourced Q4DIM map is significantly improved than those of the original Q4DIM map. The positioning error series of the original solution converges within 9 epochs to within 10 cm in the horizontal direction and 20 cm in the vertical direction, while the positioning error series of the crowdsourced solution reaches 2.3 cm in the horizontal direction and 7.6 cm in the vertical direction in 2 epochs. Compared to the original solution, the positioning accuracy of the new method improved by 48.2% in the horizontal direction and 41.2% in the vertical direction.

How to cite: Wang, B., Gu, S., Zhu, J., and Hu, J.: A Cost-Effective Crowdsourced Q4DIM Method for Rapid PPP Implementation in Wide Areas, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3961, https://doi.org/10.5194/egusphere-egu25-3961, 2025.

EGU25-7129 | ECS | PICO | G2.5

Cost-efficient dual-frequency GNSS receivers: quality assessment for geophysical applications 

Mario D'Acquisto, Markus Ramatschi, and Benjamin Männel

Lately, multi-frequency GNSS signal availability have become more commonplace, while dual-frequency receiving capability, previously restricted to expensive geodetic-grade instruments, appeared in cost-efficient and low-cost receivers. Therefore, large networks of GNSS stations with high positioning accuracy can now be deployed at limited cost, benefitting a variety of geoscience applications.

To take advantage of the developments in dual-frequency capabilites, GFZ and spin-off company maRam developed the tinyBlack GNSS receiver. The tinyBlack is compact, robust, versatile and low-power. It is equipped with one of various GNSS receiver boards and can be integrated with additional sensors. It provides a flexible, economical solution for geoscientific monitoring stations for, e.g., tectonic, volcanic and earth engineering monitoring. We evaluate the geodetic performance of different dual-frequency receiver boards in the tinyBlack.

We conduct a zero-baseline test, comparing three different receiver boards (Septentrio AsteRx-m3, Ublox  and SwiftNav Piksi) in a tinyBlack receiver and a separate, reference receiver (Septentrio PolaRx5). All boards have at least dual-frequency (L1/L2, E1/E5b) support and were simultaneously connected to a static geodetic choke-ring antenna. We first check data quality with GNut/Anubis, including observation availability, multipath linear combination, and signal-to-noise ratio. We then analyse PPP solutions with GFZ-provided precise orbits and satellite clock offsets, computing both daily and sub-daily kinematic coordinates. We compare observation residuals, coordinate estimates, and troposphere estimates. We find that the Ublox and Piksi receivers struggle more with multipath effects than the geodetic-grade receivers, despite using the same antenna in a good test location with a clear view of the sky. We also find that the Piksi has fewer observations, including a hard-coded low-elevation-angle cutoff. Probably as a consequence, it also the highest signal-to-noise ratio and lower residuals than the Piksi. PPP daily coordinate performance is vertically worse than, and horizontally comparable horizontally with, the cost-efficient receivers. Sub-daily coordinate performance is worst with the Piksi.

We also conduct a test step-wise moving antenna test to evaluate the capability of the Piksi receiver specifically to recover known displacement. We move the antenna by 5 cm every hour, alternatively forwards and backwards in a repeated 2-hour cycle, both horizontally (north-south) and vertically in separate tests. We compute kinematic PPP solutions with GFZ-provided precise orbits and clock offsets. We find that the average amplitude of the step can be recovered successfully and that both the standard deviation of the amplitudes and the scatter of coordinates at each point in the cycle is greater for the vertical component.

We finally perform data quality controls and show network-solution estimated coordinates of four GNSS stations in a field installations. The stations are co-located with seismometers installed in Italy as part of the DETECT (DEnse mulTi-paramEtriC observations and 4D high resoluTion imaging) project, which aims to acquire a dense multiparametric dataset imaging near-fault, active, slow tectonic deformation in a portion of the southern Apennines mountains with destructive historical seismicity.

In conclusion, we appreciate the developments spurred by the availability of dual-frequency signals and look forward to further field applications of dual-frequency receivers for geoscience research.

How to cite: D'Acquisto, M., Ramatschi, M., and Männel, B.: Cost-efficient dual-frequency GNSS receivers: quality assessment for geophysical applications, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7129, https://doi.org/10.5194/egusphere-egu25-7129, 2025.

EGU25-8972 | ECS | PICO | G2.5

Advancing Real-Time GNSS Applications: Performance of Galileo HAS in Precision Navigation and Low-Cost Receiver Integration 

Grzegorz Marut, Tomasz Hadas, Kamil Kazmierski, Iwona Kudłacik, and Jaroslaw Bosy

Global Navigation Satellite System (GNSS) technology, thanks to its high accuracy, is appropriate for monitoring structures, natural and anthropogenic hazards, as well as navigation and positioning. The Galileo High Accuracy Service (HAS) augmentation service recently released by the European Space Agency (ESA) is a new solution that could accelerate the development of mass-market technologies using the Global Navigation Satellite System (GNSS). Galileo HAS is designed to provide horizontal and vertical accuracies of 20 cm and 40 cm, respectively; it can be used in all legacy GNSS applications from structural monitoring to drone trajectory tracking using low-cost GNSS receivers.

This study evaluates the use of Galileo HAS with geodetic grade as well as low-cost receivers, analysing the results obtained in static, pseudo-kinematic, and kinematic solutions. The results indicate that Galileo HAS currently provides positioning accuracy at a to that comparable level of less than 10 cm, regardless of the use of geodetic or low-cost receivers. The results of integrating Galileo HAS with low-cost receivers show that it represents an important step in the development of available real-time positioning solutions.

In addition, the study showed that Galileo HAS meets key requirements in monitoring water vapour in the troposphere, as well as seismic displacement, by achieving real-time accuracy levels required for seismic displacement tracking and weather modelling. Comparative analyses with other GNSS correction streams show that HAS has lower accuracy in selected statistics, such as vertical accuracy. However, its near-global availability and high accuracy still make it a viable alternative.

How to cite: Marut, G., Hadas, T., Kazmierski, K., Kudłacik, I., and Bosy, J.: Advancing Real-Time GNSS Applications: Performance of Galileo HAS in Precision Navigation and Low-Cost Receiver Integration, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8972, https://doi.org/10.5194/egusphere-egu25-8972, 2025.

EGU25-11204 | ECS | PICO | G2.5

Improving pedestrian navigation performance with robust methods for low-cost multi-GNSS  

Sinan Birinci, Furkan Sogukkuyu, and Mehmet Halis Saka

Low-cost GNSS technology has recently expanded as an alternative to geodetic receivers in many applications, including pedestrian navigation, autonomous vehicles, atmospheric monitoring, and precision agriculture. Considering the capabilities of the receiver in terms of power consumption, size, and cost, together with the ability to record multi-GNSS observations, the low-cost receivers and patch antennas have appealed to many users. However, there exist some challenges to be addressed. Such hardware is inherently sensitive to the multipath effect, and the noise level in the observations is relatively higher, resulting in a lower carrier-to-noise density ratio (C/N0). More outliers are encountered for kinematic applications in challenging environments such as urban areas. Therefore, both realistic stochastic modeling (e.g., C/N0-dependent) and the identification of outlier observations are crucial issues for achieving reliable positioning when low-cost GNSS hardware is used. This study aims to investigate pedestrian navigation performance using low-cost GNSS and to enhance positioning accuracy through the implementation of the improved Single Point Positioning (SPP) algorithm, thanks to the code sequence. The technique employs a powerful quality control scheme to mitigate outlier observations. The method consists of two main steps: (i) If the products or measurements used for epoch-by-epoch solutions are troublesome for certain satellites, the median absolute deviation (MAD) method is applied to eliminate these observations. (ii) The remaining observations are then reweighted using a standardized residual-based Institute of Geodesy and Geophysics (IGG) III method during the least-squares. A kinematic test experiment was conducted to validate the usefulness of the approach for which observations were collected from four satellite systems with a 2-s sampling interval of approximately 20 min using a low-cost GNSS antenna (u-blox ANN-MB-00-00) and receiver (u-blox ZED-F9P). The multi-GNSS SPP solution with code observations of GPS L1, GLONASS G1, Galileo E1, and BDS-3 B1 frequencies was performed in this dataset. A GNSS station very close to the study area was used to obtain the reference trajectory with the post-process kinematic method. Analyzing only the fixed coordinates together with the corresponding SPP solution coordinates, resulted in an RMS value of about 0.50 m achieved in the horizontal component. Results showed how the utilization of proposed techniques can enhance basic SPP solutions that yield meter-level horizontal positioning accuracy. Moreover, the suggested technique improved multi-GNSS SPP solution RMS values by 33% in the horizontal and 19% in the vertical component compared with solutions without outlier detection. A comparison was also made using the findings from two distinct software packages to verify the consistency of the outcomes. The results of the evaluation indicate that the SPP algorithm exhibits comparable performance to that of the other software and validates the effectiveness of the employed technique. Finally, the GPS/GLONASS/Galileo/BDS-3 SPP, exhibiting a 3D RMS value slightly better than 2 m for pedestrian navigation, illustrates the capabilities of low-cost GNSS technology.

How to cite: Birinci, S., Sogukkuyu, F., and Saka, M. H.: Improving pedestrian navigation performance with robust methods for low-cost multi-GNSS , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11204, https://doi.org/10.5194/egusphere-egu25-11204, 2025.

EGU25-11878 | PICO | G2.5

Monitoring of geophysical deformations on a regional scale using the low-cost GNSS collaborative network CentipedeRTK  

Pierre Bosser, Julien Ancelin, Marianne Métois, Lucie Rolland, and Maurin Vidal

Developed since 2019, the CentipedeRTK network is a permanent collaborative GNSS network whose main objective is to make RTK positioning freely available, mainly using low-cost receivers and antennas. Since its creation, the network has grown considerably, well beyond the borders of France, and now includes more than 800 base stations. The main sector using the network is agriculture, but more and more public and private organisations and individuals are also using it.  

The geoscience community quickly became interested in the network, first as users of RTK positioning (for sea level monitoring, drone surveys, etc.) and then for post-processing of the raw measurements from the base stations. Since mid-2022, the RENAG network data centre has therefore been archiving the data from the base stations on a daily basis with the aim of using them for geoscience applications. A first study based on data acquired in 2023 has demonstrated the value of these data for monitoring atmospheric water vapour over continental France. 

Here we focus on the use of data acquired by CentipedeRTK base stations located in mainland France to monitor geophysical movements on a regional scale. To this end, the daily positions of the CentipedeRTK stations estimated in PPP using GipsyX are analysed and compared with those estimated for nearby permanent stations belonging to conventional networks. There is a slight deterioration in the repeatability of the mean positions (15 to 20% depending on the component). The time series show an increase in dispersion, but a very good consistency of the variations is still observed. The discrepancies observed can be explained by the equipment of the CentipedeRTK stations, in particular their antenna, as well as by the direct environment of the stations, which is not always as optimal as that of conventional stations.  

These results will be used to develop a set of recommendations for CentipedeRTK contributors and will help to increase the value of the data collected by the network's base stations for geoscience applications. 

How to cite: Bosser, P., Ancelin, J., Métois, M., Rolland, L., and Vidal, M.: Monitoring of geophysical deformations on a regional scale using the low-cost GNSS collaborative network CentipedeRTK , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11878, https://doi.org/10.5194/egusphere-egu25-11878, 2025.

In this study, we investigate the effect of antenna setup errors upon on the accuracy of position velocities produced from GNSS campaign measurements when gaps in data. Our motivation in this study is to demonstrate the changes in station velocities in time series caused by certain antenna measurement errors, in addition to the reduced frequency of data obtained from campaign-style measurements, which are preferred due to maintenance costs, permanent stations being damaged or even lost while monitoring natural events. We used seven stations from the continuous GPS time series of JPL, NASA from a global network of the IGS. For each station, we generated 1460 data for four years synthetic GNSS campaign time serieswithout gaps and 48 data with one measurement campaign per month. Subsequently, by creating data gaps through monthly campaigns, velocity estimates were made from datasets consisting of 32, 24, 16, and 8 data respectively. The same datasets were augmented with Gaussian noise simulating ±1-3 mm of antenna setup error. Velocity estimates were also made from these augmented datasets. Rms values calculated from antenna error-free datasets ranged between 0.1~0.5 mm for North, 0.2~0.5 mm for East, and 0.5~1.3 mm for Up directions. Rms values also calculated from antenna error datasets ranged between 0.2~0.9 mm for North, 0.2~0.7 mm for East, and 0.5~1.1 mm for Up directions. All velocity estimates were subjected to student t tests. About 1% variation was found for all components, both with and without antenna setup errors. The effect of antenna setup errors on data gaps in campaign-style measurements was demonstrated.

Keywords: GPS time series; GPS campaigns; Velocity estimation; Gaps in data; Antenna Setup Errors.

How to cite: Tuna, M. and Turen, Y.: The Effects of Antenna Setup Errors upon velocities of GNSS campaign measurement when gaps in data., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12633, https://doi.org/10.5194/egusphere-egu25-12633, 2025.

EGU25-14897 | ECS | PICO | G2.5

Evaluation of the ionospheric corrections generated by smartphone and application to PPP-RTK 

Yan Zhang, Yang Jiang, and Yang Gao

The ionospheric delay is a major error source in the Global Navigation Satellite System (GNSS) positioning, and its accurate estimation is essential for Precise Point Positioning Real-Time Kinematic (PPP-RTK). Traditionally, ionospheric delay estimation relies on a network of permanently deployed high-end geodetic GNSS receivers, which are costly and thus inaccessible for most consumer applications. Moreover, this approach is limited by the sparse spatial distribution and low temporal resolution of the network, leading to significant estimation errors in uncovered environments.

On the other hand, due to the global density and accessibility of low-cost GNSS receivers, such as smartphones, there is a strong demand to develop new methods for precise ionospheric delay estimation using them. Moreover, multi-frequency and multi-constellation GNSS chipsets are now embedded in smartphones including carrier phase observations essential for precise positioning. These advances support the investigation and development of new methods to enable precise real-time GNSS positioning even using smartphones. However, few studies have focused on the application and evaluation of such methods for PPP-RTK positioning.

Therefore, this study aims to develop methods to estimate ionospheric effects using low-cost GNSS receivers and demonstrate that it can provide reliable ionospheric corrections. Additionally, we evaluated ionospheric corrections using two real-time satellite orbit, clock, and code bias products, namely the satellite-based BeiDou PPP-B2b and ground-based Centre National d’Etudes Spatiales (CNES). First, the ionospheric delay estimates generated by a single reference smartphone with uncombined PPP and quality control measures based on solution separation testing is evaluated using of the real-time satellite orbit, clock, and code bias products from BeiDou PPP-B2b and CNES, respectively. Next, the generated ionospheric delay from two correction models is compared to that produced by a high-end geodetic receiver. Finally, the generated ionospheric corrections are applied to single-station-based PPP-RTK to assess its positioning performance under kinematic conditions. A field test was conducted using two Google smartphones on April 7, 2024, in Calgary. We expect to achieve decimeter-level slant ionospheric corrections accuracy compared to geodetic receiver with the two correction models used. Additionally, the positioning accuracy is expected to approach that of PPP-RTK results using geodetic receivers as base stations, significantly outperforming float PPP.

How to cite: Zhang, Y., Jiang, Y., and Gao, Y.: Evaluation of the ionospheric corrections generated by smartphone and application to PPP-RTK, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14897, https://doi.org/10.5194/egusphere-egu25-14897, 2025.

EGU25-19213 | PICO | G2.5

Positioning Accuracy of Low-Cost GNSS Systems: A Comparative Study with Geodetic Solutions 

Burak Akpinar, Cüneyt Aydin, Seda Özarpacı, Nedim Onur Aykut, Alpay Özdemir, Güldane Oku Topal, Özge Güneş, Fahri Karabulut, Efe Turan Ayruk, Hamza Çetinkaya, Muhammed Turğut, Binali Bilal Beytut, and Uğur Doğan

The increasing availability and affordability of low-cost Global Navigation Satellite System (GNSS) systems have made them a viable alternative for various geospatial applications. However, their performance and positioning accuracy require rigorous evaluation, especially when compared to geodetic-grade GNSS systems. This study investigates the accuracy of low-cost GNSS systems in positioning by comparing their results with those obtained from high-precision geodetic GNSS systems.

To evaluate the performance of low-cost GNSS systems, campaign type GNSS measurements were conducted at four points using both low-cost and geodetic GNSS systems. The collected data were processed using the Canadian Spatial Reference System Precise Point Positioning (CSRS-PPP) and the AUSPOS relative positioning services. The positioning results from these services were analyzed to assess the performance of low-cost GNSS systems relative to their geodetic counterparts. Preliminary findings indicate that low-cost GNSS systems exhibit promising accuracy levels in comparison to geodetic systems. The results highlight the potential and limitations of low-cost GNSS technology for scientific and practical applications.

This study contributes to the growing body of knowledge on low-cost GNSS technologies and provides insights into their applicability in fields such as tectonic monitoring and geodetic research. Future work will focus on refining processing techniques to further enhance the reliability of low-cost GNSS systems.

How to cite: Akpinar, B., Aydin, C., Özarpacı, S., Aykut, N. O., Özdemir, A., Oku Topal, G., Güneş, Ö., Karabulut, F., Ayruk, E. T., Çetinkaya, H., Turğut, M., Beytut, B. B., and Doğan, U.: Positioning Accuracy of Low-Cost GNSS Systems: A Comparative Study with Geodetic Solutions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19213, https://doi.org/10.5194/egusphere-egu25-19213, 2025.

EGU25-19702 | PICO | G2.5

Precise Estimation of Snow Water Equivalent based on GPS and Galileo Measurements 

Patrick Henkel, Markus Lamm, and Franziska Koch

A precise information on Snow Water Equivalent (SWE) and Liquid Water Content (LWC) is essential for various applications, e.g. for optimized operations of hydropower plants, for improved flood forecast, and for cryosphere research.
Global Navigation Satellite System (GNSS) receivers and antennas can be used to measure the snow water equivalent, snow height and liquid water content. The GNSS receivers are much more cost-effective and easy to install than other sensors such as snow scales and pillows. Our set-up consists of two GNSS receivers/ antennas, whereas one GNSS antenna is placed on the ground (i.e. below) the snow and serves as actual sensor.
The other GNSS antenna is placed on a pole above the snow and serves as reference antenna. We use the pseudorange, carrier phase and carrier to noise power ratio observables from both GPS and Galileo. The pseudorange and carrier phase measurements of both GNSS antennas are combined in double difference measurements to eliminate orbital errors, clock errors and atmospheric delays.
The snow has three effects on the GNSS signals: The first one is a time delay caused by the reduced speed of signal propagation in snow. The second effect is the refraction at the air-snow interface according to Snell's law. The third effect is the signal attenuation which is mainly driven by the LWC.
These three effects of the snow affect only the lower GNSS antenna, i.e. the double differencing does not eliminate the effects of the snow. It only eliminates the atmospheric delays being common to both GNSS antennas.
The presentation covers a precise modeling of GNSS carrier phase and pseudorange measurements, and a mathematical description of the SWE and LWC estimation from the GNSS carrier phase, pseudorange and carrier to noise power ratio measurements. We investigate different parameterizations and evaluate their impact on the SWE solution. We show the measurement results for a snow monitoring station of ANavS at an Alpine test-site for the complete previous winter period 2023/ 2024.

How to cite: Henkel, P., Lamm, M., and Koch, F.: Precise Estimation of Snow Water Equivalent based on GPS and Galileo Measurements, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19702, https://doi.org/10.5194/egusphere-egu25-19702, 2025.

EGU25-1694 | ECS | Orals | SSS9.12

Mulching improves soil-plant water status and yield in experimental drought conditions 

Jeroen Schreel, Rémy Willemet, Guillaume Blanchy, Waldo Deroo, Sarah Garré, Peter Lootens, Isabel Roldán-Ruiz, Maarten De Boever, and Tom De Swaef

Climate change-driven drought events are becoming increasingly common across Europe. These events can dramatically affect crop production, leading to significant yield losses and an overall deterioration of yield quality. Furthermore, irrigation is often not possible or allowed during long drought periods due to water scarcity. This problem requires crop management adaptations that provide more stable yields during challenging environmental conditions. To this end, organic mulch materials are being used as an agroecological solution. However, the effects of this management practice are not always straightforward, which has led to contradictory observations regarding their effect on crop yield. Here, we investigate the effect of applying an organic grass-clover mulch layer on the soil-water relations of celery (Apium graveolens Tango L.) during an extreme drought event. A full-factorial setup was used with (i) plants growing on a rainfed field with supplementary irrigation and plants subjected to drought using a movable rainout shelter and (ii) soil with and without organic mulch. Based on soil moisture and soil water potential sensors, and below-ground ERT (Electrical Resistivity Tomography) measurements, it was observed that the soil below mulched areas maintained a higher soil water content for a longer period of time compared to the soil in areas without mulch. Plant growth was monitored over time by combining manual measurements and drone data. Plants subjected to drought with mulch were significantly larger compared to plants without mulch, resulting in yields comparable to rainfed fields without mulch. Furthermore, the stomatal conductance and leaf water content of plants in mulched fields tended to be higher compared to plants in fields with no mulch. However, rainfed fields with mulch provided an even higher yield, indicating that the positive effects of the organic mulch were probably also mediated by a buffered soil temperature and an additional nitrogen input. Overall, organic mulch appears to buffer the soil-plant water relations of celery during drought, providing more stable yields under a changing climate.

How to cite: Schreel, J., Willemet, R., Blanchy, G., Deroo, W., Garré, S., Lootens, P., Roldán-Ruiz, I., De Boever, M., and De Swaef, T.: Mulching improves soil-plant water status and yield in experimental drought conditions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1694, https://doi.org/10.5194/egusphere-egu25-1694, 2025.

Tea is a globally important crop, that is highly sensitive to variations in climate. While the UK has traditionally imported tea from regions such as China, India, and Sri Lanka, there are now several tea producers established across the UK. However, the potential impacts of future climate change on the suitability of different regions of the UK for tea cultivation is currently poorly understood.

This study evaluates the future climate suitability for tea cultivation across the UK. Comparing the current climate from various continental European tea growing regions with UKCP climate projections under the four representative concentration pathway (RCP) scenarios, we analyse where in the UK European cultivars could feasibly be grown over the century. A ranking approach was employed, incorporating closeness between European current, and UK future climates, including temperature (Tmin and Tmax), precipitation, and humidity projections, to identify regions most conducive to tea growth. Results indicate that the southeast of the UK may provide optimal growing conditions in the future, contrasting with the west, where current tea farms are predominantly located.

These findings have implications for the strategic planning of tea farming in the UK, particularly due to the long lifespan of tea plants, highlighting the need for potential adaptation to shifting climate conditions such as importing cultivars that are more suitable for the future UK climate. Furthermore, the methodology offers a framework that could be extended to assess the viability of tea gardens outside the UK, and other crops under changing climatic regimes, supporting resilient agricultural practices.

How to cite: Howard, H.: Exploring the suitability of European tea cultivar growth in future UK climates., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3253, https://doi.org/10.5194/egusphere-egu25-3253, 2025.

EGU25-3287 | Orals | SSS9.12

Balancing agronomic production, farm economics and water quality with precision conservation 

Douglas Smith, Kabindra Adhikari, and Chad Hajda

Sustainable farms must balance agronomic production, farm economics and environmental concerns. Nutrient losses from agriculture are known to degrade downstream water quality. Many practices and technologies have been used to minimize the impact agriculture has on water quality, but few studies have been able to demonstrate how precision agriculture can accomplish such benefits. This presentation will demonstrate how precision agriculture was used to improve runoff water quality and farm gate returns through the adoption of precision conservation. At a research farm near Riesel, Texas, USA, ten cropped fields were managed with various levels of conservation adoption. Precision agriculture technologies were adopted for planting, fertilizing, and harvesting equipment in 2017. A baseline of data was captured from 2018-2021 to determine crop yield stability for each field. Starting in crop year 2022, the crop yield stability was used to implement precision conservation on four fields: two fields received reduced inputs to 60-80% of recommended rates in unprofitable zones, while two fields eliminated production in unprofitable zones. Water quality monitoring occurs in six of the ten fields. Preliminary data indicated decreased in soluble P loads of 90% following adoption of precision conservation, due to lower or eliminated P applications. Precision conservation seems to be able to balance production, economics and environmental concerns greater than traditional agriculture.  

How to cite: Smith, D., Adhikari, K., and Hajda, C.: Balancing agronomic production, farm economics and water quality with precision conservation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3287, https://doi.org/10.5194/egusphere-egu25-3287, 2025.

EGU25-3752 | ECS | Posters on site | SSS9.12

Climate Twin Methodology for Assessing the Future Viability of European Vineyards: A Bioclimatic and Topographic Approach 

Héloïse Allaman, Stéphane Goyette, and Jérôme Kasparian

The repercussions of climate change on viticulture are a matter of increasing concern, particularly in Europe, where vineyards are intrinsic to both the economy and cultural heritage. In order to facilitate a more profound comprehension of the spatial change of the climate, the climate twin method [1] is employed to analyse the case of European vineyards. The methodology involves the use of a climate twin model, which matches future vineyard climates with those of other regions. This provides insights into how shifting climates may influence the suitability of current and potential vineyard regions. The approach enables an understanding of both current and future climate conditions in wine-producing regions, offering prospective insights into the potential shift of suitable vineyard locations. The employment of the climate twin method facilitates the identification of regions within Europe that will retain their suitability for viticulture under future climate conditions, whilst concomitantly enabling the discovery of new areas with wine-growing potential in the future.

We rely on several bioclimatic indices, that consider climate conditions in the context of vineyard growth and disease development. The Huglin index and the number of heat and frost days are employed to describe the optimal conditions required for vine growth. The Scaphoideus titanus, the vector of Flavescence dorée, as well as the downy and powdery mildew, which are the main threats to European vineyards, are also considered. The climate twins are computed using these bioclimatic indices, as well as the raw climate data, namely temperature, precipitation, humidity and solar radiation. Results show that using the bioclimatic indices yields consistent mappings region by region, with a specific region being reliably associated with another under future climate conditions. 

Topography is a pivotal factor in viticulture, with vineyards frequently situated in hilly regions with south-facing slopes to maximise sunlight exposure. These topographic characteristics modify temperature, thereby influencing vine growth and disease dynamics. In this study, we analyse the impact of topography by calculating temperature corrections based on slope orientation and altitude. We show that the influence of these adjustments plays an important role on the identification of climate twins, and subsequent predictions for vineyard viability under future climate scenarios.

The findings of this study offer a more robust understanding of how European viticulture will need to adapt to climate change, with a particular focus on spatial shifts in suitable regions. This will assist winegrowers in making informed decisions regarding vineyard locations, culture management strategies, and future investments in viticulture. Our study underscores the significance of the climate twins approach to understanding climate impacts on viticulture, taking into account both bioclimatic variables and topographic factors. The overarching objective of this research is to provide a scientific foundation for the sustainable viticulture practices that will be required in the face of ongoing climate change, thereby safeguarding the future of European winemaking.


[1] G. Rohat, S. Goyette, J. Flacke, International Journal of Climate
Change Strategies and Management (2017)

How to cite: Allaman, H., Goyette, S., and Kasparian, J.: Climate Twin Methodology for Assessing the Future Viability of European Vineyards: A Bioclimatic and Topographic Approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3752, https://doi.org/10.5194/egusphere-egu25-3752, 2025.

EGU25-6950 | ECS | Posters on site | SSS9.12

Mulch Type Matters: The Impact of Mulch Biodegradability on Potato Crop Development Under Wet Conditions in Belgium 

Rémy Willemet, Jeroen Schreel, Tom De Swaef, Wim Cornelis, and Maarten De Boever

In Europe, future summers are expected to bring both droughts and periods of excessive rainfall, highlighting the need for adaptable agronomic strategies across varying climatic scenarios. While mulch is well-documented for its ability to reduce soil evaporation and enhance tolerance against drought, its effects under wet conditions remain unclear.

In this study, we investigated the efficacy of three types of organic mulch - hay, miscanthus, and woodchips - for potato cultivation (Solanum tuberosum L.) during the wet summer of 2024 in the Flemish region of Belgium. Mulch was applied as a 6-cm layer on a sandy loam field. To gain insights into the impact of mulching on soil processes and crop development, we measured soil water content, matric potential, temperature, microbial activity, nitrogen in both soil and plant, and crop growth through a combination of manual and UAV measurements.

Our findings indicate that mulch biodegradability was the main factor affecting crop development during the wet 2024 growing season. At the final harvest, the average tuber yields under hay and miscanthus treatments were 33.2±3.0 t/ha and 29.2±4.5 t/ha, respectively, surpassing the control group yield of 28.1±3.3 t/ha. In contrast, the woodchip treatment resulted in a lower tuber yield of 24.4±4.4 t/ha. The best-performing mulch thus led to an 18% increase in tuber yield, while the worst-performing mulch induced a 13% decrease compared to the control treatment.

We assume that rapidly decomposing mulches provided a nitrogen boost mediated by soil microbial activity, thereby enhancing crop growth. In contrast, slowly decomposing materials might have caused nitrogen immobilization, reducing crop development and yield compared to the control group. The study underscores that the effectiveness of mulching is context-dependent and shaped by the interplay of mulch characteristics, environmental conditions, and crop-specific requirements.

How to cite: Willemet, R., Schreel, J., De Swaef, T., Cornelis, W., and De Boever, M.: Mulch Type Matters: The Impact of Mulch Biodegradability on Potato Crop Development Under Wet Conditions in Belgium, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6950, https://doi.org/10.5194/egusphere-egu25-6950, 2025.

EGU25-7186 | Posters on site | SSS9.12

Telomere Length as a genomic biomarker of well-being in grapevines: preliminary results in Aglianico grapevine 

Alessandra Iannuzzi, Arturo Erbaggio, Rossella Albrizio, Filippo Accomando, Andrea Vitale, and Ramona Pistucci

In recent years, molecular biomarkers have emerged as important tools in modern agriculture, facilitating the monitoring of plant health and providing objective assessments of resistance and susceptibility to environmental factors. Within the realm of grapevines (Vitis vinifera L.), genomic biomarkers hold promise owing to their ability to integrate multifaceted, context-dependent information.

In this context, telomere length emerges as a promising, rapid, and cost-effective genomic biomarker, as observed in other species such as mammals and other plants. Telomeres, repetitive DNA sequences situated at chromosome ends, play a central role in safeguarding genetic material from damage and have been widely used in processes related to health, aging, and stress in mammalian models.

Quantitative real-time PCR (qPCR) enables precise quantification of telomere length relative to an internal reference gene specific to grapevines, ensuring stable measurements across diverse environmental conditions. Implementation of this novel protocol will facilitate the evaluation of telomere length dynamics in grapevines under varying conditions, thereby providing a valuable tool for assessing the vine's health status.

This contribution presents the first results on the Aglianico vine subjected to different levels of water stress (irrigated and non-irrigated) under the same soil in an area of southern Italy devoted to the production of high-quality wines (Taurasi DOCG area) in the Tenuta Donna Elvira winery (Montemiletto—AV).

The results were be achieved within the BeViteLo project.

How to cite: Iannuzzi, A., Erbaggio, A., Albrizio, R., Accomando, F., Vitale, A., and Pistucci, R.: Telomere Length as a genomic biomarker of well-being in grapevines: preliminary results in Aglianico grapevine, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7186, https://doi.org/10.5194/egusphere-egu25-7186, 2025.

EGU25-7215 | Orals | SSS9.12

Assessing the Impact of Climate Change on Vineyard Ripening and Water Dynamics: A Case Study from the Taurasi DOCG in Southern Italy 

Angelo Basile, Rossella Albrizio, Antonello Bonfante, Maurizio Buonanno, Roberto De Mascellis, and Marialaura Bancheri

Climate change poses long-term risks to agriculture, driven by shifts in temperature, precipitation, and increased extreme weather events. Rising temperatures shift growing seasons, while altered precipitation affects water availability. Extreme weather, including intense rainfall, increases the risk of soil erosion and runoff. These changes are particularly important for vineyards, where grape ripening timing, crucial for wine quality, is affected. Vineyards, often located in hilly regions, also face soil degradation, impacting not only production but sectors like eno-tourism.

In this study - under the AGRITECH PNRR project - an experimental vineyard at Tenuta Donna Elvira in Montemiletto (AV), located in the Taurasi DOCG district (southern Italy), was used to assess the impact of climate change on soil and vineyard dynamics. The research included the following activities: i) identifying functional homogeneous zones (fHZs) in the vineyard using lidar-derived Digital Terrain Models (DTM), electromagnetic induction (EMI) sensor data, and vegetation indices derived from UAV flights; ii) Monitoring soil water content, agro-meteorological variables, leaf water potential, and leaf area index (LAI) over two years; iii) Conducting soil analysis on two distinct but adjacent soil types, evaluating their chemical, mechanical, and hydrological properties.

For both soils, the agro-hydrological model FLOWS was first calibrated and validated. Subsequently, simulations were conducted to assess conditions under the current climate (ACT: 2016–2023), near future (NEAR: 2025–2049), mid-future (MID: 2050–2074), and far future (FAR: 2075–2099) across three climate scenarios. These scenarios were derived from datasets provided by the 6th phase of the Coupled Model Intercomparison Project (CMIP6), utilizing three General Circulation Models (GCMs)—MPI-ESM1-2-LR, MRI-ESM2-0, and GFDL-ESM4—and three Representative Concentration Pathways (RCP2.6, RCP7.0, and RCP8.5). The models were locally validated against ground data (precipitation and mean temperature) for the period 2006–2023 and bias-corrected using a linear technique with 10 years of data (2014–2023) from a weather station located approximately 10 km from the study site in Luogosano (PZ).

The results indicated that under the RCP2.6 scenario, the ripening date remains stable, while under RCP7 and RCP8.5, ripening advances by up to 6 weeks. The increase in groundwater recharge due to climate change is minimal, with an increase of less than 6% in the far future for both soils. Soil 1 is, on average, 50% more effective at preventing runoff and flooding than Soil 2. Runoff increases from the RCP2.6 scenario to the RCP7 scenario and further under the RCP8.5 scenario.

Challenges with GCMs include inconsistencies in predicting climate variables, emphasizing the need for ensemble approaches. Despite these challenges, process-based models have proven reliable for predicting agricultural outcomes, especially in managing vineyard ecosystems under climate change.

How to cite: Basile, A., Albrizio, R., Bonfante, A., Buonanno, M., De Mascellis, R., and Bancheri, M.: Assessing the Impact of Climate Change on Vineyard Ripening and Water Dynamics: A Case Study from the Taurasi DOCG in Southern Italy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7215, https://doi.org/10.5194/egusphere-egu25-7215, 2025.

The assessment of soil functions and ecosystem services requires reliable eco-physiological indicators that capture the complexity of soil processes across scales. Long-term field experiment provides unique insights into soil carbon dynamic and functions under varying agricultural management practices and environmental conditions. In this study, we plan to conduct a meta-analysis of self-obtained field data from several long-term field experiments in Bad Lauchstädt, central Germany, to evaluate the applicability of both basic and novel eco-indicators in assessing soil health and carbon sequestration.
Our analysis includes traditional indicators such as metabolic quintet (qCO2) and microbial biomass carbon to soil organic carbon ratio (MBC:SOC), alongside some potential novel indicators like active microbial fractions, particulate organic matter to soil organic matter ratio (POM/SOM), soil pore characteristics, and soil fauna. These long-term field experiments represent varying land use practices, climatic conditions, and management strategies, offering a robust dataset for testing indicator sensitivity and effectiveness.
The primary objective of this research is to identify which indicators are most responsive to land use, climate variability, and seasonality at the field scale, and to explore their potential for evaluating soil functions and ecosystem services. While our data analysis is ongoing, we hypothesize that integrating basic and novel indicators will provide a comprehensive framework for soil assessment, enabling better predictions of ecosystem resilience and carbon storage potential. We look forward to presenting our findings and discussing the implications of eco-indicator-based assessments for sustainable soil management and climate change mitigation at the conference.

How to cite: Wang, S. and Blagodatskaya, E.: Meta-analysis of soil eco-indicators to assess soil functions and ecosystem services in long-term field experiments in Bad Lauchstädt, Central Germany, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7372, https://doi.org/10.5194/egusphere-egu25-7372, 2025.

EGU25-7657 | ECS | Posters on site | SSS9.12

RICE-MAP: A Prototype Decision Support System for Climate-Informed Rice Security in Southeast Asia 

Chen Zhao, Yaomin Wang, Chao Zhang, and Xiaogang He

Southeast Asia is a cornerstone of global rice security, contributing substantially to regional and international food supply chains. Accurate and timely information on rice yield is essential for effective agricultural planning, trade policy formulation, and food security management. However, conventional approaches to yield estimation, which often rely on historical trends or sparse in situ observations, are insufficient for capturing the complex interplay between climate variability, extreme weather events, and crop dynamics. The increasing frequency and intensity of climate shocks, including droughts, floods, and heatwaves, underscore the need for an advanced rice yield forecasting system. The development of a decision support system--RICE-MAP (Rice Information & Climate Evaluation- Monitoring And Prediction), integrates state-of-the-art climate forecasts with machine learning techniques to provide dynamic, high-resolution predictions of rice yield under current and future climate scenarios. RICE-MAP synthesizes satellite-derived datasets, global climate model outputs, and agricultural statistics to monitor and predict yield variability across rice-growing regions in Southeast Asia. By leveraging spatially and temporally resolved climate variables with machine learning models, the system provides lead-time-specific yield predictions, accompanied by rigorous evaluations of forecast performance using established metrics. The system’s capabilities are accessible through a user-friendly dashboard, designed to facilitate decision-making for policymakers, agricultural planners, and other stakeholders. Case studies in Southeast Asia demonstrate the system’s potential of integrating climate science and artificial intelligence to enhance climate resilience and adaptive capacity in the agricultural.

Keywords: Decision Support System; Rice yield forecast; climate shocks.

How to cite: Zhao, C., Wang, Y., Zhang, C., and He, X.: RICE-MAP: A Prototype Decision Support System for Climate-Informed Rice Security in Southeast Asia, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7657, https://doi.org/10.5194/egusphere-egu25-7657, 2025.

The agricultural sector faces increasing pressure to meet global food demand due to population growth. Challenges such as climate change, resource scarcity, and environmental degradation will further increase this problem. These issues are particularly critical in the Mediterranean region, which is characterized by water-limited conditions and soils poor in organic matter and mineral nutrients. As a step toward ensuring food security, optimized resource utilization strategies and actionable plans for stakeholders are necessary. Reliable estimation of crop growth parameters and yield prediction under different climatic and agronomic scenarios have emerged as critical tools in driving these changes.

Various conventional crop growth parameter estimation and yield prediction methods have emerged as methods for optimizing resource utilization, identifying risks, and enabling effective decision-making. However, conventional methods, including empirical, statistical, and process-based models, often face limitations such as co-linearity among predictor variables, assumptions of stationarity, and the inability to capture complex biophysical and biochemical interactions at large scales. These shortcomings highlight the need for more robust and adaptable approaches. Advanced technologies, particularly Artificial Intelligence (AI) and Remote Sensing (RS) have revolutionized agriculture by uncovering hidden patterns, enabling large-scale monitoring, and improving prediction accuracy. This research evaluates the state-of-the-art in the synergized use of AI and RS for crop growth parameter estimation and yield prediction in Mediterranean agroecosystems.

A systematic literature review was conducted following the Preferred Reporting Items for Systematic reviews and Meta-Analyses (PRISMA) guidelines. Keywords and Boolean operators were used to search titles, abstracts, and keywords in selected databases, including Web of Science and Scopus. The review included English and French publications focusing on the Mediterranean region, encompassing Southern European, Middle Eastern, and North African countries bordering the Mediterranean Sea. Publications that were duplicated, unrelated to the study objectives, or outside the geographical focus were excluded. Out of 551 initial publications retrieved, 117 met the inclusion criteria and were selected for detailed review.

The findings reveal a rising interest in integrating AI and RS for estimating crop growth parameters and predicting yield. Multispectral RS products, such as Landsat-8 and Sentinel-2, are the most frequently utilized data sources. Additionally, Sentinel-1 microwave sensors and Unmanned Aerial Vehicle (UAV)-based imagery are increasingly employed alongside ground-based sensors. Among AI methodologies, Machine Learning (ML) algorithms like Random Forest (RF), Artificial Neural Networks (ANN), and Support Vector Machines (SVM) dominate, while Deep Learning (DL) techniques such as Convolutional Neural Networks (CNN) and Long Short-Term Memory (LSTM) networks have gained prominence since 2020. Most publications were produced between 2020 and 2024, with Italy, Spain, and France being the most studied regions.

The study underscores the transformative potential of integrating AI and RS for crop growth parameter estimation and yield prediction in Mediterranean agroecosystems. By leveraging diverse data sources, algorithms, and sensor technologies, these advancements address the limitations of traditional models, enhance scalability and accuracy, and support sustainable agriculture in resource-limited environments.

This research is performed in the framework of the PhD program in Agrobiosciences, Scuola Superiore Sant'Anna, scholarship: PNRR “Digital and environmental transitions” (M4C1, Inv. 3.4) ex MD 629/2024.

How to cite: Demissie, W., Sebastiani, L., and Rossetto, R.: Synergizing Artificial Intelligence and Remote Sensing for Enhanced Crop Growth Parameter Estimation and Yield Prediction in Mediterranean Agroecosystems: A Systematic Literature Review, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8207, https://doi.org/10.5194/egusphere-egu25-8207, 2025.

EGU25-8877 | ECS | Orals | SSS9.12

Silicon fertilizer increased potato drought tolerance and reduced soil N2O emissions in two Danish soils at field scale  

Yvonne Madegwa, Yihuai Hu, Jörg Schaller, and Klaus Butterbach-Bahl

Potatoes, with their small, shallow roots, are one of the most drought-sensitive crops. Silicon (Si) fertilizers have the potential to increase the drought tolerance of potatoes by modulating soil and plant properties. We investigated the effect of Si fertilizers on potato production and greenhouse gas emissions (N2O and CH4) under drought stress. The experiment was conducted on 2 soils (orthic haplohumod-sand and typical Agrudalf-clay) with drought intensity as main plot (acute drought and severe drought) and Si fertilizers as split plots (amorphous silica-ASi, diatomaceous earth-DE and no-Si addition-Control). For drought intensity treatments, acute drought had higher total yields compared to severe drought, while Si fertilizer treatments (ASi and DE) had higher total yields as well as higher soil moisture and leaf P content compared to the Control in both soils. Overall, Si-based fertilizers (ASi and DE) significantly reduced cumulative N₂O emissions in both sand and clay soils compared to Control treatments. More specifically Si-based fertilizers recorded an average reduction of 31% in N₂O emissions compared to Control. For CH₄ emissions, Si-based fertilizers led to an 8% increase in CH₄ uptake in clay soils and a 3% increase in sand soils (with DE) compared to Control, although these values were not significant. Our results indicate that, at field scale, Si fertilization has the potential to be a sustainable solution for maintaining potato production while reducing agricultural N2O emissions under drought stress in Denmark. 

How to cite: Madegwa, Y., Hu, Y., Schaller, J., and Butterbach-Bahl, K.: Silicon fertilizer increased potato drought tolerance and reduced soil N2O emissions in two Danish soils at field scale , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8877, https://doi.org/10.5194/egusphere-egu25-8877, 2025.

EGU25-9409 | Posters on site | SSS9.12

Neglected and underutilized plant species to enhance productivity of marginal lands in the Mediterranean basin 

Cristina Da Lio, Marta Cosma, Luna Al-Hadidi, Abdelmadjid Boufekane, Sandra Donnici, Alaa El-Din Abdin, Amal ElRawy, Lorenzo Frison, Luca Galeazzi, Taoufik Hermassi, Maria Lopez-Abelairas, Dalila Loudyi, Simona Castaldi, Micòl Mastrocicco, Luigi Tosi, Eleni Maloupa, Katerina Grigoriadou, and Vassilis Aschonitis

The Mediterranean region is experiencing severe environmental pressures due to climate change, population growth, agricultural intensification, and desertification. Impacts will be exacerbated in the coming decades and require adaptation strategies to increase the resilience of ecosystems and counteract land degradation. Throughout the Mediterranean, desertification combined with reduced freshwater availability will be the main factors limiting agricultural production, driving the need for alternative low-water demanding crops. Some Neglected and Underutilized Species (NUS), typical of the Mediterranean area and already used by rural populations, are adapted to grow under drought conditions, in combination with other soil limiting factors, such as high salinity, reduced nutrient inputs, and desertification. These species have the potential to ameliorate soil quality and to be a viable alternative for farmers, especially smallholders, to generate economic value.

The VENUS project (i.e. ConVErting marginal lands of the Mediterranean basin into productive and sustainable agroecosystems using low water demanding Neglected and Underutilized Species) aims to demonstrate the environmental potential of introducing NUS, known for their resilience under extreme conditions, and their economic potential as marketable products, including food, cosmetics, and energy applications. Specifically, 10 pilot sites have recently been established in 7 Mediterranean countries (Greece, Italy, Morocco, Tunisia, Egypt, Jordan and Algeria) to collect data on biotic and abiotic factors regulating the NUS production systems, to test the suitability and sustainability of NUS, and to assess the impact of their cultivation on soil health quality. The local results obtained at the pilot sites, combined with an analysis of the distribution of the most recent databases available in the literature of key abiotic/climatic factors across the Mediterranean, will be useful for the scalability and transferability assessment of NUS production systems to a wider scale. Furthermore, NUS production system at each site will be analysed to assess their quality for various market applications (i.e., food, cosmeceutical and pharmaceutical, and energy production), and social acceptance with the final aim of producing a set of commercially viable and sustainable business models at partners’ pilot regions and countries, providing alternatives to farmers struggling with water scarcity and other limiting factors.

Funding

This work was conducted in the framework of the project VENUS - “ConVErting marginal lands of the Mediterranean basin into productive and sustainable agroecosystems using low water demanding Neglected and Underutilized Species” funded by the PRIMA programme (Grant Agreement No. 2312) supported by the European Union’s Horizon 2020 research and innovation programme.

How to cite: Da Lio, C., Cosma, M., Al-Hadidi, L., Boufekane, A., Donnici, S., El-Din Abdin, A., ElRawy, A., Frison, L., Galeazzi, L., Hermassi, T., Lopez-Abelairas, M., Loudyi, D., Castaldi, S., Mastrocicco, M., Tosi, L., Maloupa, E., Grigoriadou, K., and Aschonitis, V.: Neglected and underutilized plant species to enhance productivity of marginal lands in the Mediterranean basin, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9409, https://doi.org/10.5194/egusphere-egu25-9409, 2025.

EGU25-9410 | ECS | Orals | SSS9.12

Integrated digital solutions for sustainable farm-scale water allocation in Mediterranean environments 

Andrea Borgo, Marta Debolini, Guido Rianna, and Simone Mereu

Agriculture represents the most water-demanding sector in the Mediterranean, constituting 72% of total water demand, but exceeding 80% in most Southern Mediterranean countries. Moreover, climate change is expected to threaten water resources, by increasing evapotranspiration rates and changing precipitation regimes, with more heavy rains and prolonged long-term droughts. For these reasons, improving irrigation efficiency through policies like the Integrated Water Resource Management (IWRM) is critical for sustainable development. The digitalization of the irrigation sector can constitute a strategic solution to overcome the issue of water scarcity, as it integrates the latest technological advancements (Internet of Things – IoT, innovative water and weather sensors and actuators) in conventional irrigation systems. For this purpose, this work aims to develop and implement a real-time irrigation model, which acts as a decision-support tool for accurate irrigation management in Mediterranean environments. By integrating sensor-based data (soil moisture sensors, water meters and weather stations), weather forecasts (from meteorological models) and user inputs (crop, soil and irrigation management indications), the irrigation model provides accurate scheduling of irrigation events, according to crop water needs. The model runs at hourly scale, performing a soil water balance over the soil profile of the field and assessing the irrigation requirements, given the inputs (precipitation and irrigation) and outputs (deep percolation and crop evapotranspiration) of the system. The model schedules the days and volumes of future irrigation events, considering the scenarios of optimal irrigation (Early), moderate (Late) and high (Limit) water stress, in the case of full and deficit irrigation. One of the key features of the presented irrigation model is its ability to calibrate future irrigation events by analyzing the performance of past irrigations and checking the presence of deep percolation or water deficit in the lowest level of the soil profile. This model can constitute a powerful tool for the support of farmers in precision irrigation, considering the real-time monitoring of crop water needs and the scheduling of future irrigation events. Moreover, its user-friendly interface, with a very limited and easy-to-get set of input data allows an accessible management and visualization of the model’s outputs. This work is part of the PRIMA-founded ACQUAOUNT (Adapting to Climate change by QUantifying optimal Allocation of water resOUrces and socio-ecoNomic inTerlinkages - https://www.acquaount.eu/ ) project, which aims to apply innovative tools, smart water services and digital solutions, to improve sustainable irrigation and contribute to climate resilience in agriculture.

How to cite: Borgo, A., Debolini, M., Rianna, G., and Mereu, S.: Integrated digital solutions for sustainable farm-scale water allocation in Mediterranean environments, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9410, https://doi.org/10.5194/egusphere-egu25-9410, 2025.

EGU25-10094 | ECS | Orals | SSS9.12

Assessment of soil health indicators in a regional strategy for climate change adaptation in agricultural land in Navarre (Spain). 

Miguel Itarte, Rodrigo Antón, Alberto Enrique, Isabel de Soto, and Iñigo Virto

Due to expected climate change effects, and with the aim of improving the resilience of the region of Navarra (N Spain), the Life Nadapta project has developed different studies on diverse knowledge fields. One of them is related to agriculture, more specifically to soil heath and the capability of improving its resilience through different agricultural managements.

These managements are conservation agriculture, organic amendments and crop rotation and the goal of this work was to assess the effect of these practices on three previously defined soil quality indicators (bulk density, water holding capacity and organic carbon storage).

To measure the effect of this practices over the agricultural soils of Navarra, previously a zonification process took place, considering the agroclimatic distribution and different bioregions. As result of this, the region of Navarra was split into 12 zones. Subsequently, for each zone, the more representative agricultural soil managements were selected in a network of more than 150 agricultural plots. On these, paired comparisons on plots with on the same soil unit and contrasting management were conducted to determine the effect of the selected management strategies on soil health.

Result of an extensive plot selection, 11 plots were chosen out of the 150 in the network to continue the study several years after the first assessment, comparing the effect of a conventional management with the adaptative ones on soil health indicators.

In addition, to account for all aspects of the sustainability of these managements in real life, the study took into consideration the economic yield and cost of each management strategy in these 11 plots.  

The groups of plots that showed significant differences in bulk density between adaptive and conventional management were those located in study zone 3 (semi-arid transition area). The plot under conservation agriculture management displayed higher values than the conventional one and the plot with organic amendments obtained a lower density.

Regarding carbon concentration, the same plot under conservation agriculture mentioned above performed worse than its conventional equivalent. On the other hand, in study area 1 (arid Mediterranean), the plot with organic amendments achieved a higher concentration than the conventional plot.

Finally, no differences were observed in any of the groups of plots studied, in terms of the water retention capacity indicator.

The economical balances showed that not all situations leading to improved soil quality resulted in a better economical behavior, which suggests that improving soil resilience may induce additional costs to producers.

Our results offer a first approximation of actual changes in agricultural fields when adaptive strategies are adopted at the regional level.

How to cite: Itarte, M., Antón, R., Enrique, A., de Soto, I., and Virto, I.: Assessment of soil health indicators in a regional strategy for climate change adaptation in agricultural land in Navarre (Spain)., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10094, https://doi.org/10.5194/egusphere-egu25-10094, 2025.

The plant pathogen Xylella fastidiosa (Xf) is a significant threat to various economically important tree cash crops. Although previously found only in the Americas, the bacterium responsible for olive quick decline syndrome was detected in Apulia, Italy, in 2013. The primary vector of Xf in Italy is the spittlebug Philaenus spumarius. Several studies suggested that vector mobility has been a critical factor influencing the epidemic, along with the insect population density and the pathogen transmission rate. Since then, it has spread to approximately 54,000 ha of olive trees in the region, causing dramatic concern throughout the Mediterranean basin. As a result, it is crucial to comprehend its distribution and forecast its potential diffusion. While a large contribution to the “olive quick decline syndrome” (OQSD) study has been focused on the insect-bacterium characteristics as well as on the climate, phenological and epidemiological Xf-driving factors, to date, the effect of the anthropogenic pressure on the distribution of OQDS has been neglected, notwithstanding some authors hinted to the importance of human mobility and settlements on the vector dissemination, and on the actual spread of insect pests over short and medium distances. To fill this research gap, we analyzed the spatiotemporal patterns of the OQDS epidemic in Apulia using an ecological niche model to identify how different land uses, used as proxies of different levels of human pressure across the Apulia territory, impacted the distribution of the Xf-infected olive trees in 2015–2021. Results demonstrated that the anthropogenic component significantly contributed to the epidemic, with the road system representing the main driver of diffusion and natural/seminatural areas hampering Xf spread at the landscape scale. This evidence highlighted the importance of explicitly considering the effects of the anthropogenic landscape when modelling Xf distribution and support the design of landscape-informed monitoring strategies to prevent Xf spread in Apulia and other Mediterranean countries.

How to cite: Raparelli, E., Bregaglio, S., and Bajocco, S.: Assessing the driving role of the anthropogenic landscape on the distribution of the Xylella fastidiosa-driven “olive quick decline syndrome” in Apulia (Italy), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10182, https://doi.org/10.5194/egusphere-egu25-10182, 2025.

Viticulture in Trentino Alto Adige (northern Italy) mainly focuses on wine quality rather than quantity, and it is well known that wine quality can be improved by applying moderate water stress during fruit ripening. But with climate change extreme drought periods are becoming more and more frequent, and longer often coupled with high air temperatures. This is challenging for farmers, since prolonged periods of water scarcity negatively affect the physiological activity of the vines, the yield and the increase of water demand from irrigation reservoirs. On the other hand, summer extreme precipitations cause, as well, crop loss, plant diseases, nutrient leaching and soil erosion. 

With appropriate precision irrigation practices the timing and the amount of water can be controlled to guarantee the optimal amount of water to the crops and ensure the best quality of the products, also avoiding water loss by runoff or deep percolation resulting from an excess of irrigation. In this perspective it is essential to accurately monitor the water status of the SPAC, which is the Soil-Plant-Atmosphere Continuum.

This study focuses on the comparison of two different irrigation regimes on a vineyard located in Mezzolombardo (Trentino Alto Adige, Italy), with the analysis of the water status of the field during the 2024 growing season and the comparison of the musts after harvest.

Four vines (Vitis vinifera L., Teroldego cv.) on the same vine row were chosen: two of them were kept without irrigation, and the others were treated as usual with irrigation scheduled by the irrigation consortia. The water state of the plant was monitored with microtensiometers (FloraPulse Co., Davis, USA) embedded in the trunk and measuring the stem water potential (Ψstem) allowing a continuous, non-invasive and remote monitoring of Ψstem. The amount of water in the soil was measured with tensiometers, located near each plant, and atmospheric parameters were given by a meteorological station nearby.

The start of the 2024 growing season has been extremely wet and limited the initial development of the vegetation, but August was characterized by almost no water income and particularly high temperatures. Despite the lack of water, the non irrigated plants never reached Ψstem values associated to water stress, whereas the irrigated plants were kept regularly irrigated even when the water in the soil was above field capacity, leading to a potential loss of water by deep percolation. The comparison of the musts between the two thesis highlighted no significant differences in the organoleptic properties and the Ravaz Index showed that the non irrigated vines were in a better vegetative-productive equilibrium with respect to the irrigated plants.

In order to adapt the agricultural production to the water imbalance given by the changing climate, it is more effective to provide irrigation only when needed, and not to rely on a scheduled calendar. It is confirmed that precision irrigation practices accurately support the crop needs and it should be one common practice to be developed and enhanced in the near future.

How to cite: Mattedi, C., Zottele, F., Centurioni, F., and Corradini, S.: Effects of deficit irrigation practices on the Soil-Plant-Atmosphere system: a case study on Vitis vinifera L. (Teroldego cv.) from Trentino Alto Adige, Italy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10812, https://doi.org/10.5194/egusphere-egu25-10812, 2025.

Grape downy mildew, caused by the pathogen Plasmopara viticola, is one of the most devastating diseases impacting grapevine cultivation globally. Its primary infection is highly influenced by weather conditions and the presence of airborne sporangia. Effective management of this disease relies on timely preventive fungicide applications, which depend on accurate forecasting. Traditional empirical forecasting methods often lack precision, leading to costly and less effective intervention decisions. Recently, the use of spore traps for monitoring airborne spores has shown promise in enhancing plant disease forecasting accuracy.

This study aims to enhance Rossi’s primary infection model and develop a spore data assimilation method to improve the forecasting of grapevine downy mildew infections. Additionally, we examine the impact of climate change on disease occurrence risks and evaluate adaptation strategies across different grape-growing regions in China. By integrating spore trap monitoring data with the mechanistic model, our data assimilation method improved primary infection predictions and disease management strategies.

From 2022 to 2024, we conducted multisite monitoring in Nanning, Hechi, Guilin, and Yangling to analyze sporangia splash patterns and concentration changes within orchards, as well as disease index variations across regions. The collected data were used for model verification and calibration. We employed data assimilation techniques and performed a model sensitivity analysis to determine relevant parameters. The enhanced model demonstrated high sensitivity, specificity, and accuracy across major grape-growing regions in China, correctly predicting primary infection dates with a coefficient of determination (R²) of 0.85 and a root mean square error (RMSE) of 8-16%. Notably, the model accurately forecasted infection dates across multiple years and sites, with only one instance of a 7-day delay. Furthermore, the model identified optimal fungicide spraying windows, potentially reducing management costs by 10-30% compared to traditional strategies used by farmers.

Our analysis of climate change scenarios revealed significant shifts in primary infection trends, with warmer and more humid conditions projected to increase the risk and frequency of downy mildew outbreaks in several key grape-growing regions. In response, we propose adaptation strategies including the adoption of resistant grapevine varieties, modification of irrigation practices to reduce humidity around plants, and the implementation of integrated pest management (IPM) approaches that combine biological control agents with optimized fungicide application schedules.

These results indicate that assimilating real-time spore counts allows the model to effectively simulate primary infection processes, enabling timely and informed decision-making to limit disease spread. Additionally, understanding the climate change-driven shifts in infection trends facilitates the development of robust adaptation strategies to sustain grapevine cultivation under evolving environmental conditions. This approach provides grape growers with location-specific, precise, and timely information essential for developing effective disease management and adaptation strategies, thereby enhancing the sustainability and productivity of grapevine cultivation in the face of climate variability.

How to cite: Yao, L., Zhao, G., Chen, B., and Yu, Q.: Optimizing Primary Infection Forecasting and Management of Grapevine Downy Mildew with Spore Trap Data Across Chinese Vineyards, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12159, https://doi.org/10.5194/egusphere-egu25-12159, 2025.

Agricultural conservation practices (e.g. conservation tillage, cover crops) are critical measures to mitigate nutrient loss and greenhouse gas emissions, enhance soil organic carbon (SOC), and maintain crop yield. Despite these benefits, recent studies indicate that switching to conservation tillage (e.g. no-till) can inadvertently increase nitrate leaching, thereby degrading water quality.  This study presents a meta-analysis of field experiments to elucidate the conflicting outcomes of conservation tillage—increasing SOC levels but simultaneously exacerbating nitrate loss. For instance, SOC in the top 30 cm of soil under no-till (NT) was 14.2% and 4.7% higher than under high-intensity tillage (HT) and intermediate-intensity tillage (IT), respectively. In contrast, nitrate leaching under NT exceeded that under HT and IT by 4.9% and 0.6%, respectively.

By leveraging high-resolution datasets of soil characteristics, weather, water quality, land use, and topography, we utilized a comprehensive watershed model, the Terrestrial-Aquatic Sciences Convergence (TASC) to evaluate the combined effects of tillage and cover crops (e.g., winter wheat, rye, and oats) on SOC sequestration, nitrate loading, and crop yield in the Upper Mississippi River Basin (492,000km2). We found that conservation tillage  and cover crops could complement each other. The combined adoption significantly affects water availability, nitrate leaching, SOC, and crop yield. While the integration of cover crops enhances biomass production and SOC, their ability to absorb soil inorganic nitrogen during the non-growing season helps mitigate nitrate leaching. Notably, crop yield under scenarios combining tillage and cover crops surpasses those involving only tillage. However, cover crops can also enhance evapotranspiration, which could potentially aggravate the water availability issues for crop production under future climate conditions. These results underscore the critical need for careful evaluation of the trade-offs between conservation tillage and cover crops when developing policies to address environmental challenges in agricultural ecosystems over the coming decades.

How to cite: Liang, K., Zhang, X., and Zhao, K.: Trade-offs of Conservation Practices in the US Corn-belt: Balancing Soil Organic Carbon, Water Quality, and Crop Yield, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12605, https://doi.org/10.5194/egusphere-egu25-12605, 2025.

EGU25-12701 | ECS | Orals | SSS9.12

Drivers of Spatial Variability in Corn Yield Sensitivity to Heat in the US Midwest 

Adarsh Raghuram and Ethan Coffel

Extreme heat is a growing threat to global agricultural production. Compound climate extremes, such as co-occurring hot and dry conditions driven by interactions between land and atmosphere, further exacerbate yield loss. Given the projected increase in such extremes, crop adaptation is becoming increasingly crucial to mitigate yield shocks and ensure food security. 

The US Midwest, responsible for about a third of global corn production, is a key region of focus. In this study, we find that the regional sensitivity of corn yields to extreme heat has shown an increasing trend over the past 6 decades. While this finding aligns with other studies indicating limited adaptation in the region, the spatial variations in sensitivity changes suggest more localized influences on crop yields. Using data from the USDA and ERA5, we explore the basis for this observed variability in sensitivity, with a particular focus on two management strategies—crop diversity and tillage practices—at the county scale to assess potential adaptation.

How to cite: Raghuram, A. and Coffel, E.: Drivers of Spatial Variability in Corn Yield Sensitivity to Heat in the US Midwest, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12701, https://doi.org/10.5194/egusphere-egu25-12701, 2025.

Europe's commitment to sustainability drives the need for agricultural practices that are more environmentally friendly. This transition emphasizes the protection of biodiversity, reduction of environmental harm, efficient use of resources, and the simultaneous preservation of farming profitability and food security. To support this shift, various agroecological strategies are being examined for their impact on both productivity and environmental sustainability.

The presentation will show the results of a systematic review of existing research on multicropping (MC) to evaluate its potential to enhance the environmental sustainability of agro-ecosystems while maintaining or even increasing food production. MC is defined as the sequential cultivation of more than one crop on the same field within approximately 12 months.

While MC is widely practiced in developing countries, in the European region agriculture largely relies on single-cropping, with some exceptions in the Mediterranean region. Climate change will likely allow a future expansion of MC systems in Europe. As a result, MC practices are expected to play a more prominent role in future European agriculture, necessitating an evaluation of their broader implications. The review analyses the current knowledge on the impacts of MC system implementation for yields, soil water availability, soil properties and biodiversity.

How to cite: Fader, M.: Evaluation of multicropping systems (sequential cultivation) from an agroecological perspective, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12931, https://doi.org/10.5194/egusphere-egu25-12931, 2025.

EGU25-13048 | ECS | Posters on site | SSS9.12

Rice N fertilization guided by plant nutritional status using proximal sensing 

Konrad Metzger, Léandre Guillod, Yvonne Fabian, and Thomas Guillaume

With warming climate, the conditions north of the alps become more favorable for growing paddy rice as a niche product to diversify the crop production, while simultaneously utilizing wetlands with their benefits for high biodiversity and the prevention of greenhouse gas emissions. However, growing paddy rice in these climatic conditions remains challenging, and therefore, the Nitrogen availability might not be a dominant limiting factor to reach the relatively low yield objectives of Swiss growers (3-4 t / ha). Here, we assess the occurrence of N deficiencies in paddy rice fields across Switzerland and the relative importance of the two main fertilizations (basal at transplantation and at panicle initiation) to reach the yield objectives. To achieve these goals, we used proximal sensing (SPAD (soil plant analysis development) and a near-infrared leaf spectrometer) to estimate the nitrogen nutrition index (NNI) as a fast and affordable method as needed for precision agriculture and targeted fertilization. We calibrated the methodology to determine N and chlorophyl critical values at panicle initiation for the short duration rice variety (Loto) grown in Switzerland. 

In nine paddy rice fields throughout Switzerland, proximal sensing measurements were done between transplantation and panicle initiation (determined as the best moment for the second application of fertilizer). In addition, in one paddy rice field we implemented an experiment consisting of four treatments: a standard practice, where the field was fertilized once at transplantation together with the plant (40 kg N/ha) and once before panicle initiation with a spreader (40 kg N/ha), zero fertilizer and two treatments of only one fertilizer application, namely one in which the fertilizer was applied with the transplantation, and one where the fertilizer was applied before panicle initiation.

Plant leaves were measured with two proximal sensing devices, (Hansatech SPAD meter and SpectraVue leaf spectrometer) before the second fertilization, and in the case of the experiment also one week after fertilizer application. In parallel, plant samples were collected to be analyzed for biomass, leaf N content and phenology.

Preliminary results of the SPAD values showed, that they tended to reach a maximum at ca. 18 ± 4 before panicle initiation, especially in the high yielding fields. In other fields, the SPAD values were much lower (ca. 9 ± 5), indicating the need for adapted fertilization even at low yield objectives.

In terms of yield, the experiment resulted in significantly different (p<0.05) grain yield differences between the treatment without fertilizer and with the two doses of fertilizer applied. The SPAD values showed significant differences after the second fertilizer application between the treatments that received the second fertilization and those who didn’t. No effect could be seen from the first fertilization in that case as the recent fertilization overrode the other differences.

This method could be used in the future to guide precision fertilization based on crop needs and to account for the high interannual variability.

How to cite: Metzger, K., Guillod, L., Fabian, Y., and Guillaume, T.: Rice N fertilization guided by plant nutritional status using proximal sensing, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13048, https://doi.org/10.5194/egusphere-egu25-13048, 2025.

EGU25-13091 | ECS | Posters on site | SSS9.12

Hydrochar as an emerging solution for soil health improvement: Insights from a pot trial 

Teresa Di Santo, Rossana Marzaioli, Elio Coppola, Giovanna Battipaglia, Simona Castaldi, Lucio Zaccariello, Maria Laura Mastellone, and Flora Angela Rutigliano

Anthropogenic soil degradation undermines essential ecosystem services such as food production, water purification, nutrient cycling and climate regulation. Unsustainable agricultural practices are among the main causes of soil degradation through pollution, soil loss and consequently lowering organic matter and nutrients. Adopting innovative solutions for agriculture soil management by adding low-decomposable organic amendments to the soil, such as hydrochar, can help reverse soil degradation. Hydrochar, derived from the hydrothermal carbonization of organic waste, may have the advantage of restoring the organic C stock in the soil, helping to mitigate climate change and improving soil health. Before using hydrochar at a large scale, a comprehensive assessment to exclude any potential adverse effects on the soil biotic community, playing a key role in the provisioning of ecosystem services, is needed.
This study, part of the interdisciplinary project ‘CHIMERA’ evaluating the impact of hydrochar on the soil-plant-atmosphere system, aims to investigate changes in the chemical and microbial properties of degraded agricultural soil following the application of hydrochar. Therefore, a controlled greenhouse experiment was conducted using pots (21 cm diameter, 16 cm height), each containing 1 kg of soil. Two types of hydrochar, produced by hydrothermal carbonization at 250 °C and 50 bar without oxygen, were tested: one derived from sewage sludge (HS) and the other from thistle (Cynara cardunculus L., HC) residues, respectively. Each hydrochar was applied at two doses (3 kg m and 6 kg m), and the resulting five treatments (four with hydrochar and one control) were assayed in five replicates. At different exposure times (from 18 to 517 days), the following soil properties were analysed: pH, total organic C (Corg) and its extractable fraction (Cext), microbial biomass (Cmic), activity (as respiration), the quotient of mineralization (qM) and genetic bacterial diversity (richness).
The results showed no toxicity to the soil microbial community; moreover, a general improvement of microbial biomass, activity and richness was observed, compared to control, at each exposure time, together with a significant decrease in qM, suggesting that C added as hydrochar was at least in part retained in soil. This ability highlights the positive hydrochar's role in improving soil structure and promoting resilience against erosion, drought and other climate-related challenges.
Our findings suggest that hydrochar could be a tool for sustainable agricultural practices in restoring degraded soils. However, the application of hydrochar on soils requires further studies to confirm these positive effects and whether these effects can be observed using hydrochar derived from other raw materials and for other soil types.

How to cite: Di Santo, T., Marzaioli, R., Coppola, E., Battipaglia, G., Castaldi, S., Zaccariello, L., Mastellone, M. L., and Rutigliano, F. A.: Hydrochar as an emerging solution for soil health improvement: Insights from a pot trial, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13091, https://doi.org/10.5194/egusphere-egu25-13091, 2025.

EGU25-13590 | ECS | Posters on site | SSS9.12

The use of remote sensing techniques to determine the nitrogen uptake by oats on highly variable sandy soils 

Aleksandra Franz, Józef Sowiński, Arkadiusz Głogowski, and Wiesław Fiałkiewicz

Abstract

Precision agriculture has become a critical approach for achieving efficient crop production while addressing the challenge of sustainable management of natural resources. A key component of precision agriculture is optimizing plant fertilization to maximize yields while minimizing environmental impact. Traditional methods of assessing plant nutritional status and fertilizer needs, such as soil and plant sampling, can be costly and time-consuming. Remote sensing techniques offer an alternative, reducing both the cost and time required for accurate fertilizer dose determination. Additionally, these methods provide more comprehensive information with higher spatial resolution.

This study aimed to investigate the potential of remote sensing techniques, specifically satellite imagery from Sentinel-2, to determine the nutritional needs of oats grown on highly heterogeneous soils. Field studies and satellite data analysis were conducted on an oats cultivation field situated on sandy soil with significant spatial heterogeneity in southwestern Poland. Observations and measurements were performed during the BBCH growth stages 12, 31, 49, 77, and 99.

Nitrogen uptake was calculated based on biomass yield and nitrogen content in crop samples taken at 40 designated points within the field. The AGRICOLUS software and Copernicus services were used for remote sensing monitoring of oats growth, while satellite images were processed at specific intervals to calculate selected remote sensing indices using QGIS software. Spectral data were used to determine indices such as NDVI, GNDVI, SAVI, EVI, NDMI, and MCARI.

The results demonstrated that soil heterogeneity had a significant impact on oats development and its nutritional requirements. Base on outcomes the linear model for N uptake was developed, where GNDVI and percentage content of sand in the soil where used for estimation of the nitrogen uptake.  The study confirmed that remote sensing, particularly the GNDVI index, is a highly effective tool for managing fertilization during the early growth stages of oats on light soils with high spatial variability. Therefore remote sensing techniques can be used for real-time monitoring of spatial variability, facilitating precision management of the crops.

Research carried out as part of the OPUS-LAP project entitled "Sustainable nitrogen fertilization for agricultural crops based on open laboratory and field experiments with integrated near-real-time hydrological modeling" (grant number: 2022/47/I/ST10/02453)

How to cite: Franz, A., Sowiński, J., Głogowski, A., and Fiałkiewicz, W.: The use of remote sensing techniques to determine the nitrogen uptake by oats on highly variable sandy soils, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13590, https://doi.org/10.5194/egusphere-egu25-13590, 2025.

EGU25-13591 | ECS | Posters on site | SSS9.12

Applying variable fertilization and irrigation to improve oats growth and reduce environmental impact 

Jagoda Radzimska, Izabela Michalak, Arkadiusz Głogowski, Wiesław Fiałkiewicz, and Bernard Gałka

Modern agriculture faces an urgent challenge of optimizing the use of fertilizers, especially nitrogen, which is essential for healthy plant growth. However, overuse of nitrogen fertilizers can lead to severe environmental consequences, including surface and groundwater contamination, soil degradation, and the release of harmful greenhouse gases. This study aims to investigate how different fertilization and irrigation strategies affect oats growth, with a particular focus on nitrogen distribution in the soil, straw, and grain, as well as the overall performance of the crop. The research was conducted under controlled conditions, both in a vegetation hall that simulated real field conditions and in actual field settings at the Lubnów Agricultural Farm, located in the Ślęganiana catchment area near Wrocław, Poland. Various fertilization doses were tested, along with several irrigation schemes designed to replicate extreme rainfall events. The simulated rainfalls of 10 mm and 20 mm were applied at intervals of 2, 4, and 6 days, reflecting the unpredictability of real-world weather patterns. Additionally, the experiment incorporated four distinct soil types with different granulometric compositions to assess how soil texture and structure influence the effectiveness of nitrogen uptake by crops and irrigation practices. This approach allowed to better understand the interactions between soil characteristics, fertilization, and irrigation in real agricultural systems. The results of this study are critical for advancing sustainable farming practices concerning future climate changes and costs of fertilizer itself. By examining key crop parameters, such as stem length, biomass, and grain weight, it was possible to gain valuable insights into how different management strategies impact overall crop productivity and nitrogen use efficiency with regard to crop production. As climate change continues to disrupt agricultural systems worldwide, optimizing fertilization and irrigation techniques will be essential to ensure food security while minimizing the environmental impact. This research not only contributes to improving oats cultivation, but also offers a broader perspective on how precision agriculture can address pressing global challenges in agriculture.

Research carried out as part of the OPUS-LAP project entitled "Sustainable nitrogen fertilization for agricultural crops based on open laboratory and field experiments with integrated near-real-time hydrological modeling" (grant number: 2022/47/I/ST10/02453).

How to cite: Radzimska, J., Michalak, I., Głogowski, A., Fiałkiewicz, W., and Gałka, B.: Applying variable fertilization and irrigation to improve oats growth and reduce environmental impact, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13591, https://doi.org/10.5194/egusphere-egu25-13591, 2025.

EGU25-13636 | ECS | Posters on site | SSS9.12

 Regenerative agriculture as a tool for combating climate change in semi-arid Mediterranean regions 

Salvadora Martínez-López, Miguel López-Torres, Maria Isabel Motos-Alarcón, Nieves Baena-Navarro, Vanesa Núñez-Gómez, María José Martínez-Sánchez, Maria de los Ángeles Esteban-Abad, Maria Luz Tudela-Serrano, Imad El-Jamaoui, Manuel Hernández-Cordoba, and Camen Pérez-Sirvent

The term 'carbon farming' is currently used as a synonym for 'regenerative agriculture', which is explicitly based on improving soil fertility and farm productivity (EU, 2021).

The final aim of the complementary agri-food plan AGROALNEXT is to favour the double transformation, digital and sustainable of the agri-food sector, in order to increase its competitiveness and achieve the climate and environmental objectives set out in the Green Pact, while guaranteeing the supply of healthy, safe, sustainable and accessible food to the population, as pursued by the EU Farm to Table Strategy. Specifically, line 4 'Circular Economy' is developed with the aim of reducing losses, emissions and waste generated by the agricultural sector, and of those that cannot be avoided, generating opportunities for exploitation and win-win processes in their management, which are technologically transformed into value for the sector, increasing the circularity of the sector.

The RECEC research project, which started on the 1st of September 2024, aims to enhance the resilience of agricultural production to the impacts of climate change through the promotion of efficient circularity. This project is founded on the POST LIFE plan of the LIFE AMDRYC4 project, which was led by the University of Murcia and concluded in 2022.

The objective of the RECEC project is to ensure, through a series of agricultural practices, that CO2 is absorbed from the atmosphere and stored in plant material and soil organic matter. In order to achieve these objectives, the present research project aims to evaluate and determine the suitability of new organic products, for which no data are available, such as plant biomass removed from the Mar Menor coast (Murcia, Spain), to improve soil structure, increase its fertility and evaluate its capacity as a CO2 sink for these marine by-products. Recent data from the Regional Ministry of Environment of the CARM reveals that between 2017 and 2022, a total of 32,920 tonnes of marine biomass were removed. Other vegetable waste (broccoli, cabbage, almond, olive, grapefruit and fig tree pruning waste) from agricultural activity in the Region of Murcia that can be used as by-products for soil regeneration have also been incorporated.

The results obtained from this research will be useful to collaborate in the governance of the implementation of the European 'Carbon Farming' Strategy. These solutions would provide a common framework for the entire national territory, and the rest of the European regulations, thereby demonstrating the potential of Mediterranean rainfed agriculture to play a significant role as a tool for climate change mitigation, as a carbon sink and as a supplier of ecosystem services. The benefits obtained from this project translate into agricultural tools for climate change mitigation and adaptation through, for example, the fight against desertification, biodiversity conservation and socio-economic benefits, which would curb rural depopulation, in line with meeting the demographic challenge.

This study formed part of the AGROALNEXT programme and was supported by MCIN with funding from European Union Next Generation EU (PRTR-C17.I1) and by Fundación Séneca with funding from Comunidad Autónoma Región de Murcia (CARM).

 

How to cite: Martínez-López, S., López-Torres, M., Motos-Alarcón, M. I., Baena-Navarro, N., Núñez-Gómez, V., Martínez-Sánchez, M. J., Esteban-Abad, M. D. L. Á., Tudela-Serrano, M. L., El-Jamaoui, I., Hernández-Cordoba, M., and Pérez-Sirvent, C.:  Regenerative agriculture as a tool for combating climate change in semi-arid Mediterranean regions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13636, https://doi.org/10.5194/egusphere-egu25-13636, 2025.

EGU25-16383 | ECS | Posters on site | SSS9.12

AquaCrop assets and regional applications 

Louise Busschaert, Gabrielle De Lannoy, Dirk Raes, Shannon de Roos, Zdenko Heyvaert, Jonas Mortelmans, Samuel Scherrer, Maxime Van den Bossche, Sujay Kumar, Elias Fereres, Margarita Garcia-Vila, Pasquale Steduto, Theodore Hsiao, Lee Heng, Maher Salman, Jaemin Eun, Vincent Deketelaere, and Michel Bechtold

AquaCrop is a relatively simple crop model with a wide range of applications at the point, field, and regional to continental scales. Its four main assets, distributed by FAO (https://www.fao.org/aquacrop/en/), are: (i) the standard program with a graphical user interface (GUI), (ii) the open-source version-controlled Fortran90 code available on GitHub, (iii) the stand-alone programs for Windows, macOS, and Linux, and (iv) its integration into systems for efficient regional-scale modeling, satellite-based data assimilation, and climate impact simulations. Specifically, a parallelized Python wrapper is available to run the stand-alone program, and the Fortran90 code is integrated into NASA’s Land Information System Framework (LISF).

This poster introduces AquaCrop's four assets and focuses on two regional-scale applications in Europe. First, we demonstrate the use of the parallelized Python wrapper in the context of a climate impact study, where we evaluated current and future maize yields. AquaCrop simulations were performed at a coarse spatial resolution (0.5°) to assess future changes in yields, and yield gaps (difference between actual and potential yield, without stresses). Second, the use of AquaCrop within NASA’s LISF is presented through a data assimilation experiment, in which AquaCrop simulations were performed at a 0.1° resolution. A generic type of C3 crop was used over the entire domain, and the crop stage lengths were parametrized using the VIIRS global land surface phenology. The uncertainty in simulations was assessed by perturbing meteorological inputs and soil moisture in the upper soil layers. To correct plant water stress, SMAP-enhanced surface soil moisture observations (9-km resolution) were assimilated using an ensemble Kalman filter. Results highlight (i) the need for careful mapping between AquaCrop-simulated and satellite-retrieved soil moisture and (ii) how small updates in soil moisture can propagate to significant changes in biomass development.

How to cite: Busschaert, L., De Lannoy, G., Raes, D., de Roos, S., Heyvaert, Z., Mortelmans, J., Scherrer, S., Van den Bossche, M., Kumar, S., Fereres, E., Garcia-Vila, M., Steduto, P., Hsiao, T., Heng, L., Salman, M., Eun, J., Deketelaere, V., and Bechtold, M.: AquaCrop assets and regional applications, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16383, https://doi.org/10.5194/egusphere-egu25-16383, 2025.

EGU25-16434 | ECS | Posters on site | SSS9.12

Assessing Water Retention Potential in Agricultural Drainage Systems in Lower Austria 

Katharina Fischer, Thomas Weninger, Abobakr Hussin, Thomas Brunner, and Peter Strauss

Agricultural drainage systems have been widely implemented to enhance crop productivity by managing excess water. However, with increasing weather extremes, including prolonged droughts and heavy precipitation, drained areas face new challenges, including the need for irrigation and a critical reassessment of water retention capabilities. Despite the importance of these systems, the extent of drained agricultural land in Austria, particularly in Lower Austria, remains largely unknown. Therefore, quantitative knowledge about the agrohydrological potential of drainage water management in the complex landscapes of Austria are urgently demanded.

This study aims to estimate the volume of water discharged through existing drainage infrastructure in agricultural regions of Lower Austria. By providing a foundational dataset, we seek to quantify the scale of drainage and evaluate its impact on soil water retention. The approach involves a two-step process. First, potentially drained agricultural areas are being identified by using existing resources such as the Austrian soil survey, cadastral soil assessments which provide spatial information on slope data, soil types, and land use.

Secondly, a raster-based water balance model is employed, using meteorological data and literature-based assumptions that attribute certain fractions of total runoff to drainage discharge. The model produces monthly estimates of drainage, emphasizing water retention beyond the vegetation period. These results are then upscaled to the identified drained areas.

Future repetitions of the model will incorporate increasing complexity, including detailed soil parameters and refined hydrological modelling techniques, such as the SWAP model. However, even initial estimations provide critical insights and serve as a starting point for understanding the interplay between drainage systems, water retention, and potential management strategies. This research underscores the importance of rethinking water management practices in agricultural systems to adapt to climate-induced challenges and improve sustainability.

How to cite: Fischer, K., Weninger, T., Hussin, A., Brunner, T., and Strauss, P.: Assessing Water Retention Potential in Agricultural Drainage Systems in Lower Austria, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16434, https://doi.org/10.5194/egusphere-egu25-16434, 2025.

EGU25-16532 | Orals | SSS9.12

Soil management to mitigate climate change-related precipitation eXtremes - SoilX 

Annelie Holzkämper, Loraine ten Damme, Tommy D'Hose, Bano Mehdi-Schulz, Johannes Pullens, Heidi Leonhard, and Katharina Meurer and the SoilX researchers

With climate change, both drought and heavy precipitation are becoming more frequent. The EJPSOIL project SoilX investigated the possibilities to mitigate impacts of such extremes on crop productivity through improved soil management practices. To do that, we applied a multidisciplinaryresearch framework. Three methodological approaches were applied to derive complementary findings on the possibilities to alleviate impacts of increasingly frequent precipitation extremes on cropping systems in Europe through adaptations in soil and crop management: (1) sampling and measurement campaigns in long-term field experiments (LTE’s) along a north-south gradient through Europe, (2) simulation experiments with an ensemble of four agro-hydrological models and the development of a new model for dynamically simulating soil structural changes, and finally (3) socio-economic interviews within regional farming communities.

From the compiled results of this project, we conclude that while soil structural improvements have potential to buffer the effects of short-term droughts on crop productivity according to hypothetical agrohydrological simulation experiments. However, the adaptation benefits realized in the contrasting field treatments of LTE’s studied in this project (i.e. organic amendments / no-till vs. conventional management) are likely to be small under current and future climatic conditions as measured differences in physical, mechanical and hydraulic properties were mostly small. This can be explained by the fact that treatments implemented in current LTE’s are often conservative (i.e. relatively small differences between contrasting treatments; often only single and not combined measures are tested). This finding calls for the introduction of new LTE treatments with greater emphasis on soil health and climate resilience. The need for more efficient management strategies to maintain and improve these soil functionalities is clearly highlighted by the results from model-based studies of climate change impacts in SoilX: climate warming contributed to the degradation of soil organic carbon resources, potentially also leading to a deterioration of the soils’ ability to infiltrate water and to retain water in the crop root zone.

Based on analyses of farmer interviews across different LTE regions in Europe, we can say that, since viewpoints on and priorities in the selection of soil management choices differ, diverse strategies to promote the uptake of soil management improvements are likely to be most successful: farmers with a strong intrinsic motivation to maintain and improve soil functionalities are most likely to respond positively to educational measures and can best be supported by regulatory frameworks supporting flexibility in the choice of measures. Farmers with a stronger focus on economic and production targets, however, may better be addressed by information campaigns highlighting possibilities for reducing production cost and increasing yield benefits in combination with regulatory frameworks that buffer against economic risks and possible additional costs.

How to cite: Holzkämper, A., ten Damme, L., D'Hose, T., Mehdi-Schulz, B., Pullens, J., Leonhard, H., and Meurer, K. and the SoilX researchers: Soil management to mitigate climate change-related precipitation eXtremes - SoilX, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16532, https://doi.org/10.5194/egusphere-egu25-16532, 2025.

EGU25-17079 | ECS | Orals | SSS9.12

How accurate are soil moisture profile sensors? – Results from a multi-sensor evaluation using a sandbox experiment  

Felix Nieberding, Johan Alexander Huisman, and Heye Reemt Bogena

Many precision farming applications rely increasingly on the near-real time provisioning of accurate root zone soil moisture measurements to enable the efficient and economical use of limited freshwater resources. Besides the established sensor manufacturers who have been around for decades, new companies are entering the market, often with a portfolio of sensors especially designed for agricultural applications. These so-called soil moisture profile sensors (SMPS) exhibit a high potential for agricultural use. Their elongated shape and the ability to measure simultaneously in different depths make them especially suitable for frequent changes of location as required during cultivation of field crops. These sensors measure the volumetric soil water content (VWC) by exploiting the highly different dielectric permittivity of the solid and liquid soil compounds.

I this study we use a sandbox experiment to determine the measurement accuracy of different SMPS under controlled moisture conditions. The sandbox is a 2 x 2 x 1.5 m container filled with well-characterized fine sand which is sealed watertight to all sides. The sandbox is equipped with a 20 cm drainage layer and the water level inside the sandbox can be controlled by pumping water in or out using piezometer tubes, which are open at the bottom in the drainage layer. The SMPS were installed into the sandbox and the measurements were compared against reference measurements using CS610 TDR probes connected to a TDR100 (Campbell Scientific) and SMT100 (TRUEBNER) measurements installed in triplicate at six different depths. The measurement accuracy of 10 different sensors were evaluated, with each sensor being tested in triplicate. Most SMPS performed with reasonable accuracy under very dry and very wet conditions. However, strong variation was observed with respect to slope, offset and spread of the measurements and non-linear behavior was observed with some SMPS in the intermediate soil moisture range. The high variability of the measurement accuracy (RMSE: 1.2 – 6.5 vol. %) highlights the importance of choosing a suitable sensor, especially for precision farming applications, where it is crucial to have accurate field data to make the best management decisions without the need for soil specific calibration.

How to cite: Nieberding, F., Huisman, J. A., and Bogena, H. R.: How accurate are soil moisture profile sensors? – Results from a multi-sensor evaluation using a sandbox experiment , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17079, https://doi.org/10.5194/egusphere-egu25-17079, 2025.

EGU25-17505 | ECS | Orals | SSS9.12

From Vine to Wine: The Relationship Between Ecoclimatic Factors and Grape Yield in Italy 

Laura Massano, Benjamin Bois, Marielle Adrian, Giorgia Fosser, and Marco Gaetani

Viticulture is a key business for Italy, significantly contributing to the country's economy and cultural heritage. Italy is the largest world wine producer, with an estimated wine production of 41.0 mhL (2024 World Wine Production - OIV First Estimates). The relationship between climate variability and wine grape yield is a critical area of research, particularly considering ongoing climate change.

This study evaluates this relationship by employing ecoclimatic indices computed on key phenological periods that are crucial for grape development and specifically tailored to the life cycle of grapevines throughout the entire growing season. These periods have been identified using a validated phenological development model that accounts for various grape varieties. In addition to examining the effects of climate variability, this research also considers the risks posed by major cryptogamic diseases that can lead to significant crop losses.

To ensure the validity and relevance of the findings, the study actively engages with growers and obtains yield data from two prominent Italian wine consortia based in Lombardy and Tuscany. This localised approach allows the specific climatic and agronomic characteristics of each region to be considered, as well as the different grape varieties grown there.

The methodology developed correlates the ecoclimatic indices with the collected grape yield data through both single and multiple regression analyses, quantifying the proportion of total yield variability that can be explained by these predictors, both individually and in combination. The findings indicate that the ecoclimatic indices account for approximately 25% to 50% of the variance in grape yield.

By presenting a novel set of ecoclimatic indices derived from contemporary knowledge of climate impacts on grapevine development, this study contributes to filling a gap in the current research framework.

How to cite: Massano, L., Bois, B., Adrian, M., Fosser, G., and Gaetani, M.: From Vine to Wine: The Relationship Between Ecoclimatic Factors and Grape Yield in Italy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17505, https://doi.org/10.5194/egusphere-egu25-17505, 2025.

EGU25-18188 | Orals | SSS9.12

Tracking in-field progression of beet virus yellows using UAS remote sensing 

Toby Waine, John Beale, James Bell, Dion Garrett, Alistair Wright, Andrew Mead, and Taro Takahashi

Across Europe sugar beet farmers are experiencing unsustainable losses due the yield impact of beet virus yellows (VY). In 2020 losses of £43 M were experienced by UK growers, with some individual losses of more than £0.5 M. High forecasts of over 67% VY incidence without control measures, triggered the use of environmentally damaging neonicotinoid seed treatment in the UK for 2022 and 2023. Sustainable management of VY requires a better understanding the risk of virus transmission from adjacent fields and field margins into sugar beet crops by the aphids that are the main vector.

A time sequence of images of sugar beet fields were collected over several weeks using a multispectral drone camera, from which several spectral indices were calculated, including mNDblue. In the 2022 season, a sample of plants within a field were inoculated with disease. In 2023, two fields were allowed to become naturally infected, with additional field sampling to directly measure the rate of infection, the presence of aphids and plant species at locations in the crop and the field margin.

2022 was a high disease pressure year where the natural infection arrived soon after inoculation and spread rapidly throughout the whole field. The frequency of observations was such that it was impossible to temporally separate the introduced and natural infections, by remote sensing, through some differences were seen on one image date for some vegetation indices, but surprisingly not in the mean value of mNDblue, between the areas around the inoculation and control sites. However, the standard deviation of mNDblue index was found to be correlated with infection rate as measured by ground sampling (R2 ≈ 0.5). This finding was confirmed in 2023 – a low disease pressure year -at Morley (R2 ≈ 0.4).

The images, ground sampling and disease testing showed that there was no reservoir of infection in the field margins and that the aphid numbers and infection rates were lower near the field margins. The presence of oilseed rape adjacent to one field did not result in any clear difference in infection rate or pattern.

How to cite: Waine, T., Beale, J., Bell, J., Garrett, D., Wright, A., Mead, A., and Takahashi, T.: Tracking in-field progression of beet virus yellows using UAS remote sensing, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18188, https://doi.org/10.5194/egusphere-egu25-18188, 2025.

EGU25-18241 | ECS | Posters on site | SSS9.12

Full-Bayesian multi-level models for crop phenology in Germany 

Friedrich Busch

Full-Bayesian multi-level models for crop phenology in Germany

Friedrich Busch – Potsdam Institute for Climate Impact Research

Effective adaptation of agriculture to climate change requires detailed insights into all components of the agricultural system. Understanding the phenological development of crops is crucial not only for making informed management decisions, such as the timing of fertilizer or pesticide application and harvest but also for assessing future weather-related risks. With climate change, the timing and duration of phenological phases are expected to shift, and the likelihood of weather extremes during these phases may increase. Therefore, comprehensive phenological models with robust representations of uncertainties are essential.
Most current phenological models rely primarily on temperature-driven development units to predict crop phenology while neglecting other potential predictors. Since phenological observations are often limited, data is typically pooled to obtain seemingly robust parameter estimates. This structural decision, in combination with neglect of input data uncertainty, can lead to overconfidence in parameter estimates.
Hierarchical Bayesian models can address these issues. By employing a multi-level interpretation of the data (partial pooling), parameter estimates for varying groups within the data can be improved. In phenological data, one critical group level is the cultivar level, which is often omitted due to the limited availability of such data. For historical phenological observations of maize grown in Germany, cultivar data is partially available. To maximize the use of this data and minimize bias caused by missing information, a data imputation scheme is applied to reconstruct missing cultivar data. Subsequently, a full Bayesian statistical phenology model is calibrated, incorporating cultivar information and individual farm location as hierarchical levels.
Since phenological observations are typically collected by the local farmers, based on visual judgment, considerable uncertainty is inherent in the data. Incorporating this uncertainty into the model structure allows for more realistic parameter estimates. Furthermore, enhancing the development unit concept by incorporating additional predictors, such as radiation and soil moisture alongside temperature, has the potential to reduce unexplained variance in the data.
Model comparison and evaluation of the trade-off between predictive power and complexity are conducted using information criteria such as WAIC and Pareto-smoothed importance sampling. This work builds on recent advances in hierarchical Bayesian phenological modeling, providing new insights into key driving factors and relevant model structures. The models are developed using the Stan programming language, optimized for Bayesian analysis, and employ state-of-the-art Bayesian parameter sampling algorithms. In conjunction with climate scenarios these models can be used to estimate future changes in the phenological development of crops.

How to cite: Busch, F.: Full-Bayesian multi-level models for crop phenology in Germany, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18241, https://doi.org/10.5194/egusphere-egu25-18241, 2025.

EGU25-18905 | Posters on site | SSS9.12

Harmonization of functional anatomical traits at the leaf and wood levels in grapevine in response to different soil and canopy management 

Veronica De Micco, Francesca Petracca, Angela Balzano, Nicola Damiano, Andrea Vitale, Arturo Erbaggio, Ilia Savo Valente, Chiara Amitrano, Maks Merela, Chiara Cirillo, and Antonello Bonfante

In the Mediterranean region, viticulture is challenged by climate change which is increasing the frequency and severity of summer drought events. Under limited water availability conditions, controlling plant hydraulics and gas exchanges is crucial for crop productivity. Functional anatomical traits at the leaf and wood levels play a fundamental role in the capability of acclimation to environmental stresses. Thus, understanding how environmental factors and cultivation practices influence such traits is fundamental, given that they establish the limits of physiological acclimation capability.

Within this framework, this study aimed to evaluate if anatomical traits at the leaf and wood levels are differently harmonized when vines are cultivated under various treatments of soil and canopy management, with possible consequences on eco-physiological behavior, growth, and productivity. The study was conducted in a vineyard at the Feudi di San Gregorio winery premises (Southern Italy), where vines of the 'Greco' cultivar were cultivated under three treatments of soil management (cover crops, natural coverage, and soil tillage) and two types of canopy management (double guyot and double guyot flipped) over a period of three years. Leaf and wood anatomy were analyzed through light and epi-fluorescence microscopy to quantify functional anatomical traits linked with the efficiency of gas exchanges and water flow. To better interpret the relations among wood anatomical traits, inter- and intra-annual environmental variability, and cultivation management, the knowledge of the precise timing of wood formation is fundamental. Therefore, xylogenesis analysis was applied too, by collecting microcores biweekly from the main stem, in order to model wood growth dynamics and relate them to climate variables.

The overall data analysis showed the degree of plasticity of the ‘Greco’ cultivar at the structural level and suggested that the combination of traits at different organ levels may influence the vines’ response to climate change also mediated by pedo-climatic and cultivation conditions.

How to cite: De Micco, V., Petracca, F., Balzano, A., Damiano, N., Vitale, A., Erbaggio, A., Savo Valente, I., Amitrano, C., Merela, M., Cirillo, C., and Bonfante, A.: Harmonization of functional anatomical traits at the leaf and wood levels in grapevine in response to different soil and canopy management, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18905, https://doi.org/10.5194/egusphere-egu25-18905, 2025.

Surface wetness (SW) is a particularly relevant variable for plant growers as it is related to the incidence of microbial and fungal diseases, as well as to fruit cracking, especially in susceptible species (e.g. Prunus avium). Although knowledge of SW quantity and duration is key to discern and predict its impact on plant health status, monitoring of this variable is still based on sensors of which the output is a simple electrical voltage, rather than a water amount. Furthermore, the intrinsic heterogeneity of canopy conditions seems to play a major role on leaf microclimate and SW.

The presented study analyzes i) the effects of radiative conditions (also affected by the presence of a rain exclusion covers) on the main structural factors affecting SW and SW duration on cherry leaves and ii) the ability of a Leaf Wetness capacitive Sensors (LWS) to represent SW on real leaves. Cherry leaves grown under 4 different environmental conditions (sunlit/shaded x covered/uncovered) were simultaneously artificially wetted to various degrees and their surface water content measured immediately or after variable drying times. The leaf growing conditions appeared to be strongly associated to some leaf structural properties, such as leaf angle, in turn influencing the SW amount and duration. Concerning the LWS, their output signal was first calibrated in respect to their actual SW. Following, the LWS ability to represent the nearby real leaves SW was analyzed. The ability of the LWS to represent real leaves largely depended on the growing conditions of the latter, highlighting the limitations related to using a single sensor type to represent canopy parts affected by intrinsic ecophysiological plasticity. The present analysis provides key findings to support assessments of microclimate, SW, SW duration and its variability on fruit trees, and in particular on cherry.

The study was funded by the PRIN CHOICE project (Optimizing CHerry physiOlogIcal performanCE through the correct choice of multifunctional covers).

How to cite: Reyes, F. and Destefanis, C.: Tree protection covers affects microclimate, leaf structural properties and the suitability of leaf wetness sensors to monitor surface wetness in cherry, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18958, https://doi.org/10.5194/egusphere-egu25-18958, 2025.

EGU25-19576 | ECS | Posters on site | SSS9.12

Multi-Temporal Electrical Conductivity and NDVI Analysis for Vineyard Functional Zone Mapping 

Andrea Vitale, Filippo Accomando, Maurizio Buonanno, Rosario Gonzalez Cascón, and Antonello Bonfante

Precise soil spatial identification and characterization is crucial for optimizing vineyard management and enhancing grape quality. Various approaches exist for characterizing spatial soil variability, all aimed at zoning and identifying areas that, despite experiencing the same climate, exhibit different crop responses and therefore require differentiated management. However, the complexity of soil-plant interactions and the dynamic nature of soil properties over time necessitates the optimization of existing zoning methodologies. For instance, electrical conductivity (EC) mapping is a common technique, but relying on single-date measurements often fails to capture the full extent of spatial and temporal soil variability, even within a single growing season. Furthermore, commonly used electromagnetic induction (EMI) instruments operate at multiple frequencies to analyze different soil depths, making it challenging to directly relate these measurements to the specific soil volume explored by plant roots. Focusing on a well-defined soil depth, even if coarsely related to the root zone, would be more relevant for plant-soil interaction studies. Identifying the optimal period for characterizing soil spatial variability is therefore a key objective.

In this context, within the Agritech National Research Center project (https://agritechcenter.it/it/),  we study the use of multi-temporal EC data, acquired with a GF Instruments CMD MiniExplorer 6L, for delineating functional homogeneous zones within an Aglianico DOC vineyard at Tenuta Donna Elvira, Grottoni (AV), Italy. The CMD MiniExplorer 6L, capable of measuring EC at up to nine depths within 2 meters by combining its horizontal and vertical dipole configurations, provided detailed soil information.

EC data were collected over five distinct days spanning from April to late August, capturing seasonal soil moisture variations. Concurrently, multi-spectral imagery was acquired using a DJI Phantom 4 RTK drone across a broader timeframe from April to late October. Normalized Difference Vegetation Index (NDVI) values were derived from the drone imagery to assess canopy vigor and variability.

A k-means clustering approach was applied to the daily EC datasets, exploring various depth combinations to generate 36 distinct clustering outputs for each acquisition date. This multi-depth approach allowed for a comprehensive assessment of soil variability at different scales. The resulting EC-derived clusters were then compared with the mean NDVI values extracted for each cluster. This comparison aimed to evaluate the relationship between soil electrical properties and vine vigor, as reflected by NDVI.

The analysis revealed a strong correlation between EC-derived clusters and NDVI, demonstrating the effectiveness of EMI measurements for differentiating soil properties relevant to vineyard performance. The study also highlighted the influence of acquisition timing on the efficacy of soil classification, identifying optimal periods and depth configurations for maximizing the differentiation of functional zones. This multi-temporal, multi-depth approach provides valuable insights for precision viticulture, enabling targeted management practices based on spatially explicit soil and canopy information. The results contribute to a better understanding of soil-vine interactions and offer a practical methodology for efficient vineyard zoning.

How to cite: Vitale, A., Accomando, F., Buonanno, M., Cascón, R. G., and Bonfante, A.: Multi-Temporal Electrical Conductivity and NDVI Analysis for Vineyard Functional Zone Mapping, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19576, https://doi.org/10.5194/egusphere-egu25-19576, 2025.

EGU25-19862 | ECS | Posters on site | SSS9.12

Photoperiod and Light Intensity Impact on Wild Edible Vegetables Performance: From Controlled Environment Agriculture to Crop Resilience 

Dimitris Papadimitriou, Chistina Moschou, Ioannis Louloudakis, Michael Sabathianakis, Ioannis Christoforakis, Ioannis Livas, Ioannis Daliakopoulos, and Thrassyvoulos Manios

Climate change and urbanisation imposes substantial challenges on the agricultural sector, leading to various environmental and food security impacts. At the same time, there is a growing demand for high-quality, year-round, fresh vegetables which drives water and natural resources overexploitation. To mitigate these pressures, high-intensity cultivation strategies such as hydroponics and controlled environment farming systems are becoming more popular. In this context, given their substantial nutritional and culinary properties, wild edible vegetables are receiving renewed attention. Considering this background, here we investigate the impact of (a) photoperiod and (b) light intensity on yield performance of the wild edible green Scolymus hispanicus L (Asteraceae), wild relative of the domesticated globe artichoke (Cynara cardunculus var. scolymus), in indoor cultivation. Four treatments were applied including (a) a long photoperiod (16 hours of light and 8 dark), (b) short photoperiod (8 hours of light and 16 dark), (c) a low light intensity (40 μmol m-2 s-1) and (d) high light intensity (240 μmol m-2 s-1), using LEDs (Samsung SMD2835, Honglitronics) at a distance of one meter above the crop. Treatments were conducted in four growth chambers with adjustable photoperiod and light intensity regimes and constant temperature and air humidity levels. In each growth chamber, 15 Scolymus hispanicus L. plants were transplanted into 10 L pots and arranged on 3 gutters at a density of 9 plants m-2. Plants were fertigated daily (modified Hoagland nutrient solution), each with an individual emitter at a flow rate of 0.4 - 0.7 L plant-1 day-1. Results indicate that long photoperiod treatment was associated with increased rosette diameter (59.9±1.8 cm), and root fresh and dry weight (31.35±2.19 and 3.65±0.4 g, respectively) while high light intensity treatment increased shoot fresh and dry weight (118.58±6.34 and 7.55±0.38 g, respectively) and edible root hardness-firmness (1288.72±32.47 g), 90 days after transplant. Based on these results, we conclude that photoperiod and light intensity optimal management can increase marketable yield and quality traits of the wild crop Scolymus hispanicus L., in soilless indoor farming systems.

This work is supported by Optimus project [Grant Agreement ATTΡ4-0356837] with the co-funding of Greece and the European Union.

Reference

Appolloni, Elisa, et al. "Beyond vegetables: effects of indoor LED light on specialized metabolite biosynthesis in medicinal and aromatic plants, edible flowers, and microgreens." Journal of the Science of Food and Agriculture 102.2 (2022): 472-487.

Bantis, F. Light Spectrum Differentially Affects the Yield and Phytochemical Content of Microgreen Vegetables in a Plant Factory. Plants 2021, 10, 2182.

Papadimitriou, Dimitrios M., et al. "Effect of moderate salinity on Golden Thistle (Scolymus hispanicus L.) grown in a soilless cropping system." Scientia Horticulturae 303 (2022): 111182.

Voutsinos-Frantzis, O.; Karavidas, I.; Liakopoulos, G.; Saitanis, C.; Savvas, D.; Ntatsi, G. Can Long Photoperiods Be Utilized to Integrate Cichorium spinosum L. into Vertical Farms? Biol. Life Sci. Forum 2023, 27, 8.

How to cite: Papadimitriou, D., Moschou, C., Louloudakis, I., Sabathianakis, M., Christoforakis, I., Livas, I., Daliakopoulos, I., and Manios, T.: Photoperiod and Light Intensity Impact on Wild Edible Vegetables Performance: From Controlled Environment Agriculture to Crop Resilience, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19862, https://doi.org/10.5194/egusphere-egu25-19862, 2025.

EGU25-20555 | ECS | Posters on site | SSS9.12

Cultivar-Specific Responses of Sweet Potato Leaf Nutritional Quality to Nitrogen Application Rate and Water Availability 

Shalin Mano, David Sampson Issaka, Gopika Shibu, Shimon Rachmilevitch, and Zipora Tietel

Sweet potato (Ipomoea batatas) is an important crop with moderate tolerance to water stress. Understanding its antioxidant properties and nutritional content under various environmental stressors is vital for optimizing their nutritional value and resilience. Antioxidants like carotenoids, anthocyanins, and polyphenols are health benefits of sweet potatoes. Although previous studies have examined the nutritional components of sweet potato leaves and roots, comparative analysis of antioxidant activity and nutritional content among different cultivars under environmental stress conditions remains limited. Our study examined the antioxidant properties and nutritional content of three sweet potato cultivars, Georgia Jet, Jasmin, and Line 11-88 (recently released by LSU AgCenter) under various environmental stresses including Control (100% Nitrogen +100% water), Nitrogen stress (60% Nitrogen + 100% water), Drought stress (100% Nitrogen + 60 water), and the Combined stress of nitrogen and water (60% Nitrogen + 60% water). Nutritional content was quantified across cultivars and treatments in the leaves. Anthocyanin content varied significantly across cultivars and treatments. Jasmin had the highest response under both nitrogen and combined stresses, Line 11-88 highest under control, and Georgia Jet remained relatively low and stable across all treatments. Flavonoid content was not significantly affected by stress treatments but was higher in Georgia Jet and Jasmin compared to Line 11-88. Polyphenol content was highest in Jasmin under Control and Combined stress but remained consistent across treatments for Georgia Jet and is generally lower content for Line 11-88. The results suggest that Jasmin is the most promising cultivar in terms of antioxidant properties, making it a potential source of nutritional and functional food in sweet potato leaves.

This study explores how nitrogen and water availability variations impact sweet potato leaves' nutritional quality. Our study shows that nitrogen and water as limiting factors can cause an increase in the nutritional content of sweet potato leaves.

How to cite: Mano, S., Issaka, D. S., Shibu, G., Rachmilevitch, S., and Tietel, Z.: Cultivar-Specific Responses of Sweet Potato Leaf Nutritional Quality to Nitrogen Application Rate and Water Availability, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20555, https://doi.org/10.5194/egusphere-egu25-20555, 2025.

EGU25-20724 | Orals | SSS9.12

Development of a selective molecularly imprinted polymer composite electrospun nanofiber sensor for a multifunctional platform for monitoring fruit tree health 

Fabrizio De Cesare, Fabricio Nicolas Molinari, Riccardo Valentini, Antonio Agresti, and Antonella Macagnano

Studying volatile compounds emitted by plants is crucial in modern agriculture, providing insights into plant health, environmental interactions, and crop management. Plant volatile organic compounds (PVOCs) act as chemical signals, facilitating communication with pollinators, herbivores, and beneficial microorganisms. Understanding PVOC dynamics helps decode plant phenology events (e.g., flowering, fruit ripening), nutritional deficiencies, stress responses, and defence mechanisms. Terpenes are a class of PVOCs emitted during distinct growth stages as well as abiotic and biotic stresses.

Monitoring PVOCs (terpenes) allows for early detection of nutrient shortages, pest infestations, and disease outbreaks, enabling targeted interventions that reduce fertiliser and pesticide use, ultimately minimising crop losses. By leveraging PVOC monitoring, farmers can optimise resource allocation, enhance crop yield and quality, and reduce environmental impact, thus promoting sustainable agroecosystem management.

The MOSSA project integrated sensor technologies into IoT-based digital platforms for plant health monitoring. This project developed distinct interconnected units for each platform:

- TREE Unit – Tracks plant physiological parameters, including water consumption, biomass growth, and leaf stability.

- VOC Unit – Detects PVOC (terpene) emissions from lemon trees to monitor stress-related emission patterns.

- Power Unit – Powers the multi-sensing platform through energy harvesting.

Two different nanotechnological approaches were hired to achieve the VOC Unit goal. Electrospinning (ES) is a key nanotechnology for developing ultra-sensitive sensors, offering advantages in production efficiency and costs. The potential of ES technology to generate nanofibrous networks with various architectures featuring excellent specific surface area and remarkable porosity was combined with the exceptional selectivity of molecular imprinting technology (MIT) characterised by typical biological recognition mechanisms (e.g. enzyme-substrate, antibody-antigene, biological receptors) to developing highly sensitive and selective VOC (terpene) sensors, specifically for limonene, a key biomarker of plant biotic and abiotic stress. These sensors demonstrated extraordinary specificity, even distinguishing between stereoselective compounds. The VOC Unit, which incorporated MIT/ES sensors for limonene detection, allowed real-time monitoring of emission dynamics from lemon trees under simulated stress conditions, such as drought and pest injuries. 

The Tree Unit monitored plant health by recording sap flow, tree growth, trunk temperature, air conditions, and incoming radiation under the canopy. Sap flow, a key indicator of transpiration and water status, was measured using heat transport as a tracer within xylem tissue. After laboratory evaluation, the HPV method was selected, using a 6-second heat pulse at ~4W power.

A 4-chip ASM Osram sensor spectrometer measured incoming radiation across 28 spectral bands. An infrared dendrometer tracked tree growth, while an improved radial increment sensor achieved 0.46 m resolution with an absolute error <10 µm. A hygrometer recorded air temperature and humidity.

The Power Unit utilised a solar energy module based on a 450 nm 3D perovskite light harvester (1.65 eV band gap)between ETL and HTL layers. The ETL, composed of compact and mesoporous TiO₂, supported crystal growth and enhanced charge extraction. This solar cell module efficiently harvested solar energy, ensuring a continuous power supply for the sensing platform.

These innovations open new possibilities for plant health monitoring, contributing to precision agriculture and enabling more sustainable and efficient agrosystem management.

How to cite: De Cesare, F., Molinari, F. N., Valentini, R., Agresti, A., and Macagnano, A.: Development of a selective molecularly imprinted polymer composite electrospun nanofiber sensor for a multifunctional platform for monitoring fruit tree health, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20724, https://doi.org/10.5194/egusphere-egu25-20724, 2025.

EGU25-21214 | Posters on site | SSS9.12

Assessing Biowaste-based Amendments for Enhancing Soil Hydraulic Properties in Arid Mediterranean Soils 

Ioannis Daliakopoulos, Marios Gaitanakis, Menno Pietersen, Ioannis Louloudakis, Dimitrios Papadimitriou, Fenia Galliou, Xiaomei Yang, and Aristeidis Koutroulis

Soil organic matter (SOM) plays a significant role in modulating soil water and therefore irrigation scheduling. This relationship is especially vital in arid regions like the Mediterranean, where both SOM and water resources are scarce and increasingly threatened by the climate crisis. Soil amendments based on agricultural biowaste (e.g., compost) or byproducts of pre-existing processes (e.g., biochar) offer a cost-effective solution to boost SOM levels. However, because of this less strictly managed production process, the variability in their properties and their long-term effects on soil hydraulic behaviour, particularly after weathering, remain poorly understood. Here we compare the effect of 3 soil amendment treatments to the hydraulic properties of clay loam soil: olive tree pruning compost at 1% (C1B0), biowaste-based biochar from at 1% (C0B1), and compost-biochar mix at 1% (C1B1) against a control treatment (C0B0). Amendments were incorporated in the soil at the prescribed rates to a depth of 15 cm. To quantify the impact of the amendments in hydraulic properties of soil such as clay loam we use a modification of the hydraulic property (HYPROP2, Meter, USA) analyser (Daliakopoulos et al., 2021) after application, and 6 months after application. The assessed van Genuchten parameters are used to estimate the movement of water soil in the soil profile with HYDRUS-1D (Kool & Van Genuchten, 1991) using two distinct profiles. Simulations were validated through irrigation experiments using in-situ soil moisture measurements at 2 depths (10 and 30 cm). As shown by changes Van Genuchten parameters, results show that, compared to compost applications, biochar had a more pronounced and lasting positive effect regarding soil porosity and structure, also decreasing hydraulic conductivity and increasing field capacity. These results highlight the potential of biochar and it’s mixes to improve soil water status and contribute to the reversal of desertification processes in arid Mediterranean soils.

Acknowledgements

This work has received funding from REACT4MED: Inclusive Outscaling of Agro-Ecosystem Restoration Actions for the Mediterranean. The REACT4MED Project (grant agreement 2122) is funded by PRIMA, a program supported by Horizon 2020. MP was supported by ERASMUS+ KA131 mobility (ID 1174266). Authors IND and AK thank MINERVA Ltd. and research project “Assessment of climate change impacts on olive oil production and implementation of sustainable agricultural adaptation practices in Greece” for its support.

References

Daliakopoulos, I., Papadimitriou, D., & Manios, T. (2021). Improving the efficiency of HYPROP by controlling temperature and air flow. EGU General Assembly Conference Abstracts, EGU21--13082.

Kool, J., & Van Genuchten, M. T. (1991). HYDRUS: One-dimensional Variably Saturated Flow and Transport Model, Including Hysteresis and Root Water Uptake, Version 3.31. US Salinity Laboratory.

 

How to cite: Daliakopoulos, I., Gaitanakis, M., Pietersen, M., Louloudakis, I., Papadimitriou, D., Galliou, F., Yang, X., and Koutroulis, A.: Assessing Biowaste-based Amendments for Enhancing Soil Hydraulic Properties in Arid Mediterranean Soils, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21214, https://doi.org/10.5194/egusphere-egu25-21214, 2025.

EGU25-21391 | Orals | SSS9.12 | Highlight

CAVA: a user-driven climate service for the assessment of risks in the agriculture sector 

Rodrigo Manzanas, Riccardo Soldan, Hideki Kanamaru, Daniel San Martín, Max Tuni, Iván Sánchez, Ezequiel Cimadevilla, Josipa Milovac, and José Manuel Gutiérrez

 

Climate change impacts agricultural production globally, affecting food security and economic development at all scales. The Climate and Agriculture risk Visualization and Assessment (CAVA) framework has been co-designed by the University of Cantabria, Predictia Intelligent Data Solutions and the Food and Agriculture Organization (FAO) of the United Nations in response to the need for evidence-based climate information in formulating climate change adaptation projects (e.g. Green Climate Fund) and investment plans in the agriculture sector. 

Within this framework, CAVA Platform has been designed as a climate service which provides users with an easy access to state-of-the-art climate information through a web portal, with the aim to facilitate the assessment of risks in the agricultural sector at regional, national, and sub-national scales. In particular, this is done based on global gridded observations, reanalysis, and the ensemble of CORDEX-CORE simulations covering the period up to 2100. The tool provides immediate access to essential climate variables (temperatures, precipitation, wind, humidity, radiation), and a series of pre-computed climate-derived indices relevant to agriculture (e.g., number of days below/above temperature thresholds, number and length of dry/wet spells, frequency and intensity of heat waves, etc.), allowing the user to select his/her region, period and season of interest. Moreover, users are also allowed to conduct more sophisticated analyses on demand; e.g. by modifying the thresholds that define the aforementioned indicators, focusing on specific crops, etc. In addition, all this information can be downloaded via automatic reports. 

Concurrently to the CAVA Platform, CAVA Analytics is a cloud-based service that allows users with basic programming skills to access, process, and visualize most of the data CAVA Platform builds on. This computing environment, which is available via a web browser, relies on a Jupyter hub with a pre-installed version of the R package CAVAanalytics (https://github.com/Risk-Team/CAVAanalytics), which internally builds on the climate4R (https://github.com/SantanderMetGroup/climate4R) suite. 

How to cite: Manzanas, R., Soldan, R., Kanamaru, H., San Martín, D., Tuni, M., Sánchez, I., Cimadevilla, E., Milovac, J., and Gutiérrez, J. M.: CAVA: a user-driven climate service for the assessment of risks in the agriculture sector, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21391, https://doi.org/10.5194/egusphere-egu25-21391, 2025.

EGU25-21543 | Orals | SSS9.12

Agro-environmental Potential of Novel Organic Fertilizers Derived from Fishery Waste  

Jingsi Zhang, Çağrı Akyol, Hongzhen Luo, Stefaan De Neve, and Erik Meers

The application of novel organic fertilizers derived from secondary raw materials has emerged as a promising  sustainable agricultural practice in recent years. This study investigates the potential of organic fertilizers produced from fishery waste to be applied as alternatives for synthetic nitrogen (N) fertilizers through comprehensive soil incubation and pot experiments. The N content of eight selected organic fertilizers ranged from 1.9% to 9.8%, in which some of them were rich in labile N such as protein fractions and amino acids. In a 120-day incubation trial, six of these labile N-rich organic fertilizers demonstrated a superior mineralization rate of 49-66% compared to 10-35% for the other fertilizing products, showcasing a high concentration of readily degradable N fractions. This increased mineralization led to enhanced N availability for crop, which is crucial for short-term agricultural productivity. Remarkably, when applied to spinach at a fertilization rate of 170 kg N ha⁻¹, the tested organic fertilizers performed comparably to the synthetic fertilizer, resulting in similar yields and statistically non-significant differences in N use efficiency over two months of spinach growth. Additionally, a follow-up experiment assessed greenhouse gas emissions, especially N₂O, from soils amended with the fertilizers under high-water condition. Notably, solid organic fertilizers exhibited lower N₂O emissions (0.5%-2.0%) compared to the liquid ones (2.6%-4.5%) even when soil moisture content reached 70% of water-filled pore space, which in line with the previous field studies (Aguilera et al., 2013), where solid organic fertilizers emitted less N2O than the liquid organic fertilizers ). Overall, these circular fertilizers matched the N-supplying efficacy of synthetic fertilizers, offering a sustainable alternative. Notably, solid organic fertilizers outperformed the liquid ones in terms of N2O emissions, highlighting their potential for more environmentally friendly agricultural practices.

 

Keywords: fishery waste; organic fertilizer; nitrogen mineralization; greenhouse gas emissions

 

Reference

Aguilera, E., Lassaletta, L., Sanz-Cobena, A., Garnier, J., Vallejo, A., 2013. The potential of organic fertilizers and water management to reduce N2O emissions in Mediterranean climate cropping systems. A review. Agriculture, Ecosystems & Environment 164, 32-52.https://doi.org/10.1016/j.agee.2012.09.006.

How to cite: Zhang, J., Akyol, Ç., Luo, H., De Neve, S., and Meers, E.: Agro-environmental Potential of Novel Organic Fertilizers Derived from Fishery Waste , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21543, https://doi.org/10.5194/egusphere-egu25-21543, 2025.

EGU25-1266 | Posters on site | AS5.8

First deployment of a drone-borne active AirCore in a volcanic plume at Mount Etna 

Tanja Schuck, Johannes Degen, Nicole Bobrowski, Mélisende Bossard, Lucie Boucher, Huilin Chen, Bastien Geil, Giovanni Giuffrida, Steven van Heuven, Thorsten Hoffmann, Gianluigi Ortenzi, and Andreas Engel

Uncrewed Aircraft Systems (UAS) are by now established platforms for measurements in volcanic plumes. Trace gases of interest range from sulfur dioxide and halogenated substances to carbonaceous trace gases including carbon monoxide (CO) and carbon dioxide (CO2). However, sophisticated measurement techniques for high-precision observations of trace gases often require instrumentation that cannot be used on board UAS due to the high weight and power consumption of the devices

Originally developed for stratospheric observations, air sampling with long coiled tubes in AirCores, has proven to be a light-weight sampling technique to probe parts of the atmosphere that are otherwise difficult to access. Trace gas analysis of sampled air is done post-flight, most commonly with fast high-precision optical methods, delivering high-quality and high-resolution trace gas mixing ratios. While balloon-borne AirCore setups perform so-called passive sampling, making use of natural pressure differences, in 2018, a team at Groningen University developed a UAS-deployable small active AirCore device collecting air with a small pump.

In July 2024, we deployed this AirCore setup on a UAS to probe the volcanic plume of Mt. Etna (Sicily, Italy), which was particularly active at the time of the measurements. This was to our knowledge the first time that the AirCore sampling technique was used to sample air inside a volcanic plume. The air sample was successfully analysed with cavity-ring down spectroscopy for CO, CO2 and methane (CH4). While CO and CO2 mixing ratios were markedly enhanced in the plume and signals correlated well with SO2 enhancements observed by an electro-chemical sensor, no significant enhancement of CH4 was observed. The observed trace gas mixing ratios will be used in further studies to model the chemistry in the plume of Mt. Etna.

How to cite: Schuck, T., Degen, J., Bobrowski, N., Bossard, M., Boucher, L., Chen, H., Geil, B., Giuffrida, G., van Heuven, S., Hoffmann, T., Ortenzi, G., and Engel, A.: First deployment of a drone-borne active AirCore in a volcanic plume at Mount Etna, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1266, https://doi.org/10.5194/egusphere-egu25-1266, 2025.

EGU25-4415 | ECS | Orals | AS5.8

Cloud Sampling with UAS during the #CHOPIN Campaign at Mount Helmos in October 2024 

Anna Voss, Alkistis Papetta, Franco Marenco, Spyros Bezantakos, Marine Goret, Leo Håkansson, Konstantinos Michailidis, George Biskos, Maria Kezoudi, Nikolaos Mihalopoulos, and Jean Sciare

Uncrewed Aircraft Systems (UAS) have gained a strong presence in atmospheric sciences in recent years due to their flexibility, cost-effectiveness, and ability to access areas that are challenging for manned aircraft. As part of the #CHOPIN (CleanCloud Helmos OrograPhic Site ExperimeNt) campaign, the Unmanned Systems Research Laboratory (USRL) of the Cyprus Institute deployed UAS on Mt. Helmos, Greece, from October 11 to November 1, 2024, providing valuable data for the study of clouds.  

The #CHOPIN campaign, conducted in collaboration with NCSR Demokritos and FORTH/EPFL, was hosted at the Kalavryta Ski Center with a base altitude for the UAS takeoffs and landings of 1690 m ASL. The campaign aimed to improve the understanding of aerosol-cloud interactions and to evaluate remote sensing algorithms and models. Located in a rapidly changing "climate hotspot" at the intersection of various air masses, Mount Helmos is particularly sensitive to environmental changes, with interactions between wildfire smoke, pollution, sea salt, and Saharan dust. This unique setting provides an ideal location to study the dynamics of aerosol-cloud interactions.

This study presents an overview of the UAS operations held at Mount Helmos, highlighting collection of vertical profiles of particle size distribution from the ground (1.7km ASL) up to 3.5 km ASL, both inside and outside the clouds. In contrast to point measurements from ground-based stations, UAS can follow cloud movement and sample the entirety of the cloud, capturing aerosol particle size distributions below, within, and above the clouds, and cloud droplet size-distributions. These measurements provide valuable insights into aerosol properties and cloud-aerosol interactions at different altitudes. Additionally, consecutive UAS flights helped study the evolution of the Boundary Layer Height (BLH) at the Helmos site. The data collected can fill the vertical resolution gap of aerosol size distributions and provide additional datasets for comparison with fixed station observations. 

How to cite: Voss, A., Papetta, A., Marenco, F., Bezantakos, S., Goret, M., Håkansson, L., Michailidis, K., Biskos, G., Kezoudi, M., Mihalopoulos, N., and Sciare, J.: Cloud Sampling with UAS during the #CHOPIN Campaign at Mount Helmos in October 2024, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4415, https://doi.org/10.5194/egusphere-egu25-4415, 2025.

EGU25-4488 | Posters on site | AS5.8

Added value of off-the-shelf UAS for exploring Alpine valley flows 

Alexander Gohm

Scanning Doppler wind lidars have become an important tool for investigating the kinematic structure of the mountain boundary layer and associated local flows. However, currently, no appropriate remote sensing technique exist that can capture the thermodynamic structure (temperature and humidity) in the lowest hectometres above ground at a sufficient spatiotemporal resolution. Hence, uncrewed aircraft systems (UAS) have become a prominent tool to fill this gap.

In this work, we report how a single off-the-shelf UAS (DJI Mini 2) equipped with a temperature and humidity logger (iMet-XQ2) can provide added value for the interpretation of Doppler wind lidar observations of complex winds in a narrow Alpine valley. The study site is located at Nafingalm, a mountain pasture located at the end of the Weer Valley in Tyrol, Austria. This location will be one of the target areas of the TEAMx Observational Campaign (TOC) in summer 2025. We present data from a short campaign conducted on 01 and 02 September 2023 to test the feasibility of combined UAS and Doppler lidar measurements at this remote site. The UAS performed vertical profiles over more than 24 hours of the lowest 120 m above ground at a 30-minute interval during daytime and an hourly interval during nighttime to capture the whole boundary layer evolution.

We will show the characteristics of daytime upvalley and nighttime downvalley winds as captured by the Doppler wind lidar and the corresponding temperature structure depicted by the UAS observations. In this context, the UAS measurements were crucial for correctly interpreting the transient warming phases during early evening as turbulent mixing events resulting from the interaction of a cross-mountain airflow with the stable boundary layer in the valley. The observations indicate that the early evening transition phase is characterized by high complexity and presents an interesting phase for studying turbulent processes in more detail within the framework of the TOC.

How to cite: Gohm, A.: Added value of off-the-shelf UAS for exploring Alpine valley flows, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4488, https://doi.org/10.5194/egusphere-egu25-4488, 2025.

EGU25-4779 | Posters on site | AS5.8

Towards sensible heat flux measurements with multicopter UAS 

Norman Wildmann and Laszlo Györy

This study demonstrates the feasibility of measuring temperature variance and sensible heat flux with self-calibrated fine-wire platinum resistance thermometers (FWPRT) on multicopter drones. The sensors are especially designed for light-weight, fast response-times and to be carried on miniature drones for turbulence measurements.
A significant improvement was found in vertical profiling of temperature gradients compared to slower solid-state sensors, demonstrating reduced hysteresis between ascent and descent phases and accurate representation of strong gradients. 
More than 100 single flights with the sensors attached to drones of the SWUF-3D fleet were carried out in vicinity to a meteorological mast array at the WiValdi wind energy research park in Northern Germany. The comparison to sonic anemometers shows that mean temperature and temperature variance can be accurately measured within the background flow variability. The same applies for sensible heat flux, which was measured for the first time with multicopter UAS and the eddy covariance method. An uncertainty of 50 W m-2 was determined with the constraint that only low wind speed conditions could be used to guarantee accurate vertical wind speed measurements. The results indicate that the temperature sensors are suited for sensible heat flux measurements, but further improvements are necessary with regard to vertical wind speed estimates to decrease the overall uncertainty.

How to cite: Wildmann, N. and Györy, L.: Towards sensible heat flux measurements with multicopter UAS, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4779, https://doi.org/10.5194/egusphere-egu25-4779, 2025.

EGU25-5595 | ECS | Posters on site | AS5.8

UAV-based methodologies for quantifying methane emissions from point sources 

Abdullah Bolek, Martin Heimann, and Mathias Göckede

Uncrewed aerial vehicles (UAVs) are increasingly becoming complementary monitoring tools in various scientific fields, particularly in atmospheric and climate science, as they are versatile, relatively cheap, and can provide data at various spatial scales. However, UAV-based methodologies are still in their early stages and require extensive effort to fully exploit the potential of UAVs. Accurate quantification of emission rates from point or localized sources, such as geologic seeps or oil and gas production sites, is important for understanding emission processes and mitigating climate change. Conventional greenhouse gas monitoring platforms (i.e., flux chambers and eddy-covariance towers) have a significant sampling gap as they struggle to provide the spatial extent needed to accurately estimate emission rates from point or localized sources. UAV platforms carrying greenhouse gas analyzers for CO2 and CH4, along with an anemometer to measure 2D wind speed, air temperature, humidity, and pressure, allow capturing the spatial extent of a plume originating from a point source, and therefore accurately quantify its source strength.

The UAV platform employed for this study was used to sample a geological methane seep located in the Mackenzie Delta, Canada. Geological methane seeps can act as super emitters, releasing methane at rates significantly higher than typical biogenic sources; hence, accurate quantification of their emission rates is crucial to estimate the overall CH4 budget of the area. In July 2024, different flight strategies were tested to monitor point sources, including several curtain flights and a grid flight conducted at varying downwind distances from the seep. Using these flight data, the emission rate of the methane seep was quantified using two different methods: a mass-balance approach and a Gaussian plume inversion technique. The CH4 plume released from the seep showed concentrations about ten times higher than the atmospheric CH4 background levels, underscoring the significant potential impact of the geological seeps on the overall Arctic carbon budget.

How to cite: Bolek, A., Heimann, M., and Göckede, M.: UAV-based methodologies for quantifying methane emissions from point sources, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5595, https://doi.org/10.5194/egusphere-egu25-5595, 2025.

EGU25-6449 | ECS | Orals | AS5.8

Development of an airborne Eddy covariance system dedicated to greenhouse gases (CO2/CH4) and energy fluxes measurements of heterogeneous landscapes onboard fixed-wing UAV 

Ngoc Minh Hoang, Jean-Louis Bonne, Nicolas Dumelié, Florian Parent, Vincent Moncourtois, Grégory Albora, Jérémie Burgalat, Thomas Lauvaux, Charbel Abdallah, Pedro-Henrique Herig-Coimbra, Benjamin Loubet, Ludovic Donnat, and Lilian Joly

Climate change poses significant threats to ecosystems and human activities, necessitating urgent efforts to reduce greenhouse gas emissions. This requires new tools able to monitor and quantify emissions at the meso-scale, applicable to large industrial facilities, agricultural sites, landfills or natural areas such as forests or peatlands. To address this challenge, our project aims at developing a lightweight (< 4 kg) eddy covariance (EC) system embarked on a fixed-wing vertical take-off and landing (VTOL) uncrewed aircraft system, enabling precise measurements of greenhouse gases (CO2, CH4) and energy fluxes between the surface and the atmosphere over large and heterogeneous areas. 

The system combines a five-hole turbulence probe (ADP) to measure three-dimensional wind and air temperature, along with a custom-fabricated diode laser spectrometer for CO2, CH4 and H2O concentrations. The gas analyzer is lightweight (2.1 kg), highly accurate (< 0.5 %), capable of rapid measurements (100 Hz) and optimized for high-speed mobile platforms. 

A preliminary mobile EC system (comprising the ADP, a reference sonic anemometer and the custom gas analyzer) was mounted on a vehicular platform to evaluate the integrated sensor suite under real atmospheric conditions. Comparative analyses of instantaneous relative velocity components and turbulence spectra show close agreement between the two wind sensors, confirming the ADP’s suitability for integration into our VTOL-based EC system. Furthermore, the water vapor and CO2 concentration spectra indicate that the concentration sensor is well-suited for measuring atmospheric gases within a mobile EC setup. A continuous wavelet transform approach was applied to compute surface fluxes on agricultural fields near the road trip. Combined with a footprint analysis to study landscape heterogeneity, this lays the groundwork for a transition to a drone-based EC system.  

A flight maneuver was conducted with the ADP-equipped VTOL under unstable atmospheric conditions to validate wind and air temperature measurements. Spectral analysis indicates that the airborne platform can capture actual atmospheric turbulence. Sensible heat flux was computed for this test flight, demonstrating our drone-based EC system’s potential to generate surface fluxes and emissions maps over heterogeneous landscapes. 

As part of our future work, flight trials will be carried out to measure greenhouse gases (CO2 and CH4) and energy fluxes. These measurements will be compared against tower-based EC fluxes to evaluate the performance of the UAV-based system. 

How to cite: Hoang, N. M., Bonne, J.-L., Dumelié, N., Parent, F., Moncourtois, V., Albora, G., Burgalat, J., Lauvaux, T., Abdallah, C., Herig-Coimbra, P.-H., Loubet, B., Donnat, L., and Joly, L.: Development of an airborne Eddy covariance system dedicated to greenhouse gases (CO2/CH4) and energy fluxes measurements of heterogeneous landscapes onboard fixed-wing UAV, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6449, https://doi.org/10.5194/egusphere-egu25-6449, 2025.

EGU25-9080 | ECS | Orals | AS5.8

Quantifying methane emissions from UK Landfills Using Unmanned Aerial Vehicles 

Maria Tsivlidou, Jamie McQuilkin, Hugo Ricketts, Kieran Wood, Han Yong, and Grant Allen

Methane (CH₄) is a potent greenhouse gas, with a global warming potential 27.2 to 29.8 times greater than carbon dioxide (CO₂) over a 100-year timescale. Accurate quantification of methane emissions is crucial for developing effective climate change mitigation strategies and meeting international agreements on greenhouse gas reduction. However, significant uncertainties remain in estimating methane emissions, particularly from anthropogenic sources such as landfills, due to spatial heterogeneity and complex atmospheric interactions.

Landfills are known as significant contributors to anthropogenic methane emissions. In recent years, the use of unmanned aerial vehicles (UAVs) equipped with high-precision methane sensors has developed into a promising approach for quantifying these emissions. This method offers advantages such as improved spatial coverage, reduced operational costs and dynamic monitoring. The field of emissions quantification by UAV survey has rapidly expanded over the past decade, with a growing international academic community refining and validating methods, and an emerging commercial sector driving technological advancements.

Our study focuses on quantifying methane emissions from three UK landfills in 2024/25 using drone-based spatial sampling of in situ gas concentrations, wind speed and direction. We apply and compare different mass balance methods with varying approaches to spatial interpolation, to test the sensitivity of emission quantification to the selected approach. This analysis aims to assess the strengths and limitations of each method when applied to landfill environments. Additionally, we conduct an error analysis, examining the main sources of uncertainty such as wind measurements and background methane concentrations. 

By addressing these challenges, our research contributes to improving the accuracy and robustness of drone-based methane quantification for landfill applications (and similar local scale sources). This work supports the development of methods for measuring emissions directly, which is crucial for setting emission reduction targets and improving national greenhouse gas inventories in waste management.

How to cite: Tsivlidou, M., McQuilkin, J., Ricketts, H., Wood, K., Yong, H., and Allen, G.: Quantifying methane emissions from UK Landfills Using Unmanned Aerial Vehicles, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9080, https://doi.org/10.5194/egusphere-egu25-9080, 2025.

EGU25-9677 | ECS | Posters on site | AS5.8

Improving the accuracy of particle concentration measurements of an optical particle counter (UCASS) for balloon soundings 

Sina Jost, Ralf Weigel, Konrad Kandler, Luis Valero, Jessica Girdwood, Chris Stopford, Warren Stanley, Luca K. Eichhorn, Christian von Glahn, and Holger Tost

Since the Earth's energy balance is also influenced by aerosols and cloud droplets, knowledge concerning their size, number and vertical distribution is essential. To enable frequent, continuous, and cost-effective observations, a balloon-borne optical particle counter (“Universal Cloud and Aerosol Sounding System” (UCASS)) was developed by the University of Hertfordshire (UK). Hitherto, GPS or pressure-based measurements of the balloon’s ascent rate have been used to calculate the air’s flow velocity and volume flow rate through the UCASS, from which aerosol and cloud droplet concentrations were obtained. However, it appeared reasonable to modify the UCASS set-up by directly measuring the flow velocity in the immediate vicinity of the particle detection region within the UCASS with the aid of a thermal flow sensor (TFS), such that the volume flow within the UCASS can be measured continuously and in real time.

Consequently, a modification of the UCASS instrument has been conducted, including an internal TFS within the instrument for a more accurate determination of the probed (analyzed) air volume. This study shows that the TFS, located in a UCASS extending housing, has negligible influence on the flow velocity in the detection region within the UCASS. Field tests (in the framework of “TPChange”, DFG TRR301) have demonstrated that the ascent rates derived from GPS and pressure rarely match the TFS-based ascent rates and deviate by up to 30 %. Laboratory experiments show that with an isoaxial flow (between 2 and 8 m/s) towards the UACSS, the flow velocity within the UCASS is generally increased by ~11.3 % compared to the external flow velocity. Only if the angle of attack of the UCASS is changed to values between 20°-30°, the flow velocities within the UCASS correspond approximately to the external flow. In contrast to GPS and pressure-based ascent rates, the TFS-measured volume flow within the UCASS allows for obtaining true volume flow rates despite flow distortions (caused by the UCASS housing) and in particular the deflection of the UCASS body from an isoaxial orientation. In this way, the UCASS extension including the TFS represents an improvement of the UCASS measurements in the sense of more accurate recordings of volume flows and, thus, particle concentrations up to 7.5 km altitude.

How to cite: Jost, S., Weigel, R., Kandler, K., Valero, L., Girdwood, J., Stopford, C., Stanley, W., Eichhorn, L. K., von Glahn, C., and Tost, H.: Improving the accuracy of particle concentration measurements of an optical particle counter (UCASS) for balloon soundings, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9677, https://doi.org/10.5194/egusphere-egu25-9677, 2025.

EGU25-9787 | Posters on site | AS5.8

Using uncrewed aerial systems for investigating the vertical aerosol particle distribution close to German airports 

Lutz Bretschneider, Anna Voß, Barbara Harm-Altstädter, Konrad Bärfuss, Ralf Käthner, Falk Pätzold, Andreas Schlerf, Malte Schuchard, Markus Hermann, Ulf Winkler, and Astrid Lampert

Ultrafine aerosol particles (UFP, particles < 100 nm diameter) can contribute to respiratory and cardiovascular diseases. Aircraft engines have been found to emit significant amounts of UFP. The vertical and horizontal distribution of these particles in the vicinity of airports depends mainly on the wind speed, the local wind direction and the stability of the atmospheric boundary layer (ABL). To investigate the vertical distribution of UFP emissions depending on these parameters, TU Braunschweig conducted measurement flights with the uncrewed aerial system (UAS) ALADINA near the Berlin Brandenburg Airport (BER) in October 2021 during the ULTRAFLEB project and near the Frankfurt Airport (FRA) in October 2024 as part of the SOURCE FFR project.
During the two field campaigns, 140 and 110 vertical profiles were conducted at BER and FRA, respectively, at varying periods during the day. The results indicate that UFP concentrations are higher compared to the background conditions downwind of the airport plume. This behaviour can also be seen in the preliminary data analysis of the FRA campaign. During stable conditions of the ABL, the measured UFP remain within the inversion layer, as vertical mixing is suppressed. This is also the case for the relatively larger particles with a size diameter between 300 and 500 nm, which were mainly emitted from car traffic close to the site.
The UAS measurements performed downwind of FRA provide a profound understanding of the vertical distribution of UFP and the interaction with meteorological conditions will allow to relate this results to the in parallel performed particle dispersion and wake vortex modeling.

Acknowledgement:
This research is part of the project ULTRAFLEB (DE: Ultrafeinstaubbelastung durch Flughäfen in Berlin; EN: UFP caused by airports in Berlin) and is funded by the German Environment Agency (Umweltbundesamt) under grant RE FOPLAN FKZ 3720 52 201 0 and the work was carried out as part of the UFP exposure study SOURCE FFR (Study On Ultrafine Particles in the Frankfurt Airport Region) commissioned by the Umwelt und Nachbarschaftshaus (UNH).

How to cite: Bretschneider, L., Voß, A., Harm-Altstädter, B., Bärfuss, K., Käthner, R., Pätzold, F., Schlerf, A., Schuchard, M., Hermann, M., Winkler, U., and Lampert, A.: Using uncrewed aerial systems for investigating the vertical aerosol particle distribution close to German airports, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9787, https://doi.org/10.5194/egusphere-egu25-9787, 2025.

EGU25-11744 | ECS | Posters on site | AS5.8

Enhancing High Resolution Atmospheric Profiling Using UAS: Deployment and Validation of the PARASITE Sensor Package 

Yann Büchau, Martin Schön, Kjell zum Berge, Samantha Gallatin, Jens Bange, and Andreas Platis

Uncrewed Aircraft Systems (UAS) are an invaluable tool for atmospheric profiling due to their mobility and capability to operate in the lower atmosphere and boundary layer. These regions represent an observational gap between ground-based stations and remote sensing instruments and satellites, which tend to be less accurate at lower altitudes. To fill this gap, while prioritising usability, versatility and safety, we have developed a custom meteorological sensor suite integrated into commercially available UAS, specifically multicopters.

The custom sensor package, called the Portable Aircraft Rucksack for Atmospheric Sensing and In-situ Turbulence Estimation (PARASITE), integrates data from the aircraft's positioning system and external meteorological sensors, including fast measurement of temperature, relative humidity and barometric pressure. We demonstrated the capabilities of this sensor package in flight on a DJI Mavic 3 multicopter with dimensions of 350 mm × 290 mm and a total take-off weight of 1 kg.

The three-dimensional wind vector is calculated using an improved method that combines a physical model based on meteorological and aircraft data - such as attitude, rotor frequencies, ground speed and air density - with machine learning techniques. The accuracy of the system was validated during the VITAL field campaign against ground-based in situ and remote sensing instruments, including Doppler wind lidars, differential absorption lidar, a 120 m meteorological tower and radiosondes.

The VITAL campaign was organised by the Hans-Ertel Centre for Weather Research of the German Weather Service (DWD) at Forschungszentrum Jülich, Germany in August 2024 and was also part of the World Meteorological Organisation's (WMO) global UAS Demonstration Campaign. During the campaign, PARASITE collected more than 100 vertical profiles, which were automatically transmitted wirelessly to a central data server after landing.

The system demonstrated compliance with WMO requirements by delivering processed data products in BUFR (Binary Universal Form for the Representation of Meteorological Data) format within minutes of each flight. The PARASITE system's rapid data processing and reliable performance highlight its potential to advance atmospheric profiling and support global meteorological initiatives.

 

How to cite: Büchau, Y., Schön, M., zum Berge, K., Gallatin, S., Bange, J., and Platis, A.: Enhancing High Resolution Atmospheric Profiling Using UAS: Deployment and Validation of the PARASITE Sensor Package, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11744, https://doi.org/10.5194/egusphere-egu25-11744, 2025.

EGU25-11881 | ECS | Posters on site | AS5.8

Combined measurement of Saharan dust, meteorological variables and space charge with the uncrewed aircraft system MASC-3 over Cyprus 

Martin Schön, Vasilieos Savvakis, Matteo Bramati, Andreas Platis, and Jens Bange

Mineral dust, especially Saharan dust, has a significant impact on atmospheric processes by influencing radiative forcing and cloud formation. To improve the representation of dust events in numerical weather prediction models, high-resolution in-situ measurements are required. In this study, the MASC-3 unmanned aircraft system (UAS) was used to perform simultaneous vertical profiling of meteorological variables, turbulence, aerosol particles and space charge during an intense dust event over Cyprus in April 2022. The UAS, equipped with an optical particle counter payload (OPC-Pod), provided high-resolution measurements of aerosol number concentration, with observed peaks of 45 counts/ml at 2500 m above sea level (a.s.l.), consistent with concurrent remote sensing observations, satellite imagery and back-trajectory simulations, as well as measurements from other UAS. The space charge distribution within the dust layer showed distinct patterns at the upper and lower boundaries, consistent with theoretical expectations. This study demonstrates the capability of MASC-3 for simultaneous meteorological, aerosol and charge measurements at altitudes up to 5500 m, providing valuable data for improving dust transport models. The results highlight the value of in-situ observations with UAS in characterising the vertical structure and electrical properties of dust layers, contributing to a more accurate understanding of dust-atmosphere interactions.The measurements were part of a project supported by the European Commission under the Horizon 2020 - Research and Innovation Framework Programme, H2020-INFRADEV-2019-2, Grant Agreement number: 871115.

How to cite: Schön, M., Savvakis, V., Bramati, M., Platis, A., and Bange, J.: Combined measurement of Saharan dust, meteorological variables and space charge with the uncrewed aircraft system MASC-3 over Cyprus, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11881, https://doi.org/10.5194/egusphere-egu25-11881, 2025.

In support of obtaining accurate, high-resolution meteorological and climatological observations, over remote regions, uncrewed stratospheric platforms are a potential breakthrough in capability in support of improving weather forecasting of extreme weather events. They offer cost effective and unique observations using micro-dropsondes. They can profile the entire atmospheric column from the lower stratosphere to sea-level with high vertical resolution data.

Voltitude Ltd., uses long endurance micro-high-altitude balloons (mHAB) and is developing fixed-wing solar electric stratospheric drones, also known as High Altitude Pseudo Satellites (HAPS), for delivering and dispensing micro-dropsondes over remote regions. The new micro-dropsonde has been compared with profiles from market leading radiosondes and other dropsonde systems and offers high quality data products featuring extremely high vertical resolution. The presentation “Dropsondes from the Stratosphere” will review the global weather observation challenges, priority use cases, and how new stratospheric technological innovations are impacting this field and will discuss the emerging capabilities offered by low-cost long endurance stratospheric platforms.

Results from resent weather observation data gathering field trials using the StratoSonde® mHAB system will be presented. This is a lightweight (<3kg) self-navigating, long endurance stratospheric balloon incorporating a dispenser containing up to ten, 20g, micro-dropsondes. This mHAB is capable of accurate altitude control and can target specific wind layers to drift in desired directions towards data sparse regions of interest, with its payload of micro-dropsondes. Once dispensed the dropsondes take approximately 20-minutes to descend to sea-level, measuring Temperature, Pressure, Relative Humidity, Wind speed and Wind Direction in high vertical resolution all the way from stratosphere to sea-level. Data is transmitted to the dispensing balloon, which disseminates this in near-real-time via SATCOM. Presentation of results will include 2023 and 2024 field campaigns across the tropical Atlantic, operating out of the Cabo Verde islands, off the west coast of Africa. This valuable in-situ data is permitting new research relating to potential intensity and the role of the outflow layer in the rarely observed upper troposphere, in structural evolution and intensification of tropical cyclones.  More recently, mHAB have been deployed from Iceland to navigate to arctic regions, gathering polar observations from the 2024-2025 season, and supporting research into high latitude, short lived and intense polar low phenomena.

The presentation will conclude with results from new research into reducing the vulnerability of fixed-wing solar electric drones a.k.a. High-Altitude Pseudo Satellites (HAPS), to gusts and turbulence. The new “Gust Alleviation” technique has successfully expanded the operating envelope of HAPS for launch, recovery and flight through the troposphere to and from the relative safety of the stratosphere. This is a key enabling technology and permits HAPS to take-off and land more frequently, to enable new applications including micro-dropsonde delivery from the stratosphere, where it is critical to be able to land and restock the dropsonde payload every couple of weeks. This disruptive new capability is highly complementary to wide area, high density services currently offered by lighter-than-air mHAB and provides a higher value targeted observation of specific meteorological features of interest.

How to cite: Stevens, P.: Dropsondes from the Stratosphere: Targeted Observations Over Remote Regions Using Uncrewed Stratospheric Platforms., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13017, https://doi.org/10.5194/egusphere-egu25-13017, 2025.

EGU25-13819 | ECS | Orals | AS5.8

Max PlanckWinDarts: High-resolution measurements in the planteray boundarylayer with a tethered balloon 

Venecia Chávez-Medina, Hossein Khodamoradi, Eberhard Bodenschatz, and Gholamhossein Bagheri

Uncrewed Aircraft Systems (UAS) and tethered balloon systems (TBS) are transforming atmospheric research by enabling high-resolution, multi-instrument observations. To address long-standing gaps in planetary boundary layer (PBL) observations, particularly in the mixed layer and entrainment zone, we employed the Max Planck CloudKite, a tethered kite-balloon hybrid system, equipped with the latest generation of WinDarts. These versatile instruments provide continuous multi-parameter measurements of PBL dynamics for up to 20 hours. Each WinDart measures three-dimensional wind velocity, temperature, relative humidity, pressure, particle concentration (0.3–40 μm), carbon dioxide, and volatile organic compounds, offering unparalleled insights into PBL processes.

During the Pallas Cloud Experiment (September 2022) and the IMPACT campaign ("In-situ Measurement of Particles, Atmosphere, Cloud and Turbulence," May–June 2024) in Pallas, Finland, we deployed successive generations of WinDarts, achieving a cumulative flight time of nearly 370 hours. These campaigns yielded high-resolution datasets capturing turbulent fluxes of heat and momentum and interactions between the PBL and the free atmosphere.

This contribution presents findings from the IMPACT campaign, focusing on velocity-temperature interactions and their role in turbulence and vertical transport. The results demonstrate the value of TBS-based platforms in complementing UAS systems for atmospheric research and advancing our understanding of PBL processes.

To the left, the image shows two kite-balloons deployed with three WinDarts during a flight as part of the IMPACT field campaign. To the right, we show a lateral visualization of a WinDart highlighting its different components.

How to cite: Chávez-Medina, V., Khodamoradi, H., Bodenschatz, E., and Bagheri, G.: Max PlanckWinDarts: High-resolution measurements in the planteray boundarylayer with a tethered balloon, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13819, https://doi.org/10.5194/egusphere-egu25-13819, 2025.

EGU25-14053 | Posters on site | AS5.8

Tethered Helikite Observatories 

Eberhard Bodenschatz and Gholamhossein Bagheri

 It is impossible to build measurement towers that are several kilometers high. Traditionally, aircraft have been used for atmospheric measurements. Due to their high true air speed, time-resolved measurements from manned aircraft are very challenging. This is especially true for measurements in clouds. Dropsondes and sounding balloons are regularly used to measure atmospheric profiles. However, it is not possible to measure the transport properties of moisture, temperature and aerosols. Unmanned aerial vehicles and drones can be used to measure atmospheric properties. However, due to either the high true air speed or the downwash from the propeller system, measurements of 3D wind speed are quite limited. In addition, the payload of these systems is modest. It is impossible to measure for many hours or days.  It would therefore be desirable to have a system that can serve the same purpose as a tower, but can reach heights of several kilometers. 

In this talk I will present the Max Planck Cloud Kite Observatory. It is a tethered helikite system operated from a winch on the ground or from a research vessel. The tether holding the helikite is made of very low weight, high or low density pre-stretched polyethylene. The helikite is both a helium balloon and a kite. By this it is not pushed towards the ground at high windspeeds nor does it fall to the ground when the wind stops. By mounting two 250m^3 helikites on top of each other, we achieved a safe lift of 150kg on the tether. Remotely operated instruments can be easily mounted anywhere on the tether.  The system is certified for wind speeds up to 25m/s. Due to its stationary location it has shown to supplement measurements with UAVs perfectly.   In addition multiple tethered helikite observatories can be employed in close vicinity to each other. In other words, the Max Planck Cloud Kite is a mobile observatory platform with the same utility as a multi kilometer high tower.

 I will present the system: winch, helikite, mounting strategies, the helium recovery system and the instruments we have developed to measure eddy covariances, aerosols, and cloud particle dynamics by holographic particle image velocimetry. I will give an outlook on how such a system can be used to highly resolve stratocumulus clouds and other situations. 

 

How to cite: Bodenschatz, E. and Bagheri, G.: Tethered Helikite Observatories, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14053, https://doi.org/10.5194/egusphere-egu25-14053, 2025.

EGU25-15058 | Orals | AS5.8

Improving weather forecasts through an operational network of Meteomatics Meteodrones 

Fabiola Ramelli, Lukas Hammerschmidt, Brad Guay, Melanie Kobras, Julie Thérèse Villinger, Johannes Rausch, Lukas Umek, and Martin Fengler

Weather significantly impacts a wide range of industries and influences many aspects of our daily lives. However, weather models often lack sufficient and reliable observations in the atmospheric boundary layer, which limits their accuracy, particularly in forecasting local weather phenomena over complex terrain. To fill this observational gap, Meteomatics has developed the Meteodrone-Meteobase-system.

Meteodrones are hexacopters equipped with meteorological sensors that collect high-resolution vertical profiles of temperature, humidity, wind speed and wind direction up to 6000 meters AMSL. The Meteobase acts as a base station, enabling the automatic launch and landing of the Meteodrones. Since 2020, Meteomatics has been operating a growing network of 3-10 Meteobase stations across Switzerland that is remotely controlled by a pilot. The data collected by the Meteodrones is automatically integrated into our high-resolution weather model EURO1k (1 km2 resolution), to close the observational gap and improve weather forecasts. Building on the success and experience gained from the Swiss network, Meteomatics will install and deploy a network of 30 Meteobase stations across Norway between 2024 and 2027.

Here we assess the quality of the Meteodrone measurements against the World Meteorological Organization's (WMO) observation requirements for high-resolution numerical weather prediction. Furthermore, we evaluate the impact of the Meteodrone data on forecasting local weather phenomena, such as stratus clouds, by comparing observations to model simulations with and without assimilated drone data. These findings showcase the operational capabilities of automatic Meteodrones for meteorological profiling and its contribution to improving numerical weather forecasts.

How to cite: Ramelli, F., Hammerschmidt, L., Guay, B., Kobras, M., Villinger, J. T., Rausch, J., Umek, L., and Fengler, M.: Improving weather forecasts through an operational network of Meteomatics Meteodrones, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15058, https://doi.org/10.5194/egusphere-egu25-15058, 2025.

EGU25-17032 | ECS | Orals | AS5.8

Real-time identification of flow structures in the atmospheric boundary layer using UAV-borne measurements and neural networks 

Louis Alsteens, Matthieu Duponcheel, and Philippe Chatelain

The accurate identification and classification of wind structures in the atmospheric boundary layer (ABL) are promising to address the challenges of surface fluxes estimations and improving our understanding of the atmosphere dynamics. Traditionally, the Eddy-Covariance method is used to estimate those fluxes but it struggles to achieve the energy balance closure in specific atmospheric conditions such as day-time convective conditions. Those inaccuracies are possibly due to the presence of localized wind structures such as updrafts or other coherent structures in the vicinity of the measurement tower.

The present study was performed on numerical simulation databases to develop the methodology and will be applied to field data in the upcoming future.

First, an innovative framework that combines real-time data acquisition using unmanned aerial vehicle (UAVs) and signal reconstruction via Fourier mode decomposition is going to be presented. The UAV is flying on a predefined path to gather measurements that are then used to reconstruct the velocity field based on a limited number of Fourier modes. The solenoidal constraint is applied to the velocity field to get more accurate results. The determination of the Fourier modes is handled as a minimization problem while the limited number of modes ensures a good computational efficiency while trying to preserve the key features of the flow. The time-history of the measurements is considered up to a certain sample age but the location of the samples from the past is advected in a Lagrangian fashion according to the reconstructed field. This reconstruction process is performed in near real-time which is critical for practical applications.

Second, we will focus on the identification of the flow structures. It is handled by a neural network trained on an extensive data sets of more than 100 million samples taken from Large Eddy Simulations (LES) of convective boundary layer with various atmospheric conditions (mean Temperature going from 15 to 25°, geostrophic wind speed ranging from 0 to 4m/s...). This neural network has demonstrated good performance reaching an accuracy of 84% in structure identification according to the classification of Park et al. [1], even for ABL conditions unseen during the training process. These results showcase the robustness of the neural network and its ability to adapt to varying convective scenarios and its ability to identify various structures such as updrafts, downdraft and other coherent structures.

Finally, the two approaches are combined. Within a LES flow flied, a virtual UAV takes measurements on a predefined path, reconstructs the velocity field based on the Fourier modes approach and identifies the structures. The results of the identification problem are then compared to the actual features in the LES in order to evaluate the accuracy and effectiveness of the combined method.

[1] Park, S., P. Gentine, K. Schneider, and M. Farge, 2016: Coherent Structures in the Boundary and Cloud Layers: Role of Updrafts, Subsiding Shells, and Environmental Subsidence. J. Atmos. Sci.73, 1789–1814, https://doi.org/10.1175/JAS-D-15-0240.1.

How to cite: Alsteens, L., Duponcheel, M., and Chatelain, P.: Real-time identification of flow structures in the atmospheric boundary layer using UAV-borne measurements and neural networks, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17032, https://doi.org/10.5194/egusphere-egu25-17032, 2025.

EGU25-17544 | ECS | Orals | AS5.8

Hovering a Microscope on a Drone: Development of UAV Based Systems for High-resolution Imaging of Falling Snow 

Koen Muller, Mario Camenzind, Ilja Shesterikov, Simone Morandi, and Filippo Coletti

From single crystal formation high in the atmosphere down to precipitating snowfalls at ground level no snowflake takes the same path through the air column. During descent snow-crystals grow, coalesce, break, and rime into graupel while interacting with the surrounding air. Among the well-studied effects of temperature and humidity super-saturation, the specific role of the various turbulence activities throughout the atmosphere remains elusive. This work uses uncrewed aerial vehicles (UAVs) as a flexible platform to study snowfall up to 120 meters above ground level during their most ‘turbulent end-of-lifetime’ as they descend through the atmospheric surface layer. The work is twofold. Firstly, a smaller commercially available DJI Mavic3E quadcopter equipped with an onboard telelens and CZZI GL10 searchlight is used to gather aerial photography of snowfall 3 meters away from the drone. Automated flight paths executed in an hourly deployment scan the air column and harvest 13407 snowflakes from 3351 images taken during nighttime experiments. Building on previous ground-imaging studies, we extract snowflake metrics for size, aspect ratio, complexity, and orientation angle at a 160μm-per-pixel image resolution. Our data suggests that snowflakes of high aspect ratio tend to glide in horizontal orientation while interacting with the turbulent atmosphere. Mapping our data over various height positions we find an overall 30% percent variability in snowflake growth, while variation in shape is found less prominent. Secondly, we present developments on an airborne microscopy system to shed further light on the intricate details of the snowflakes concerning their freefall behavior. Equipping a larger DJI Matrice600Pro hexacopter capable of carrying a 6kg payload with an Infinity K2-Distamax long-range microscope telescopic lens we increase the image resolution by a factor of ten and reach 16μm-per-pixel. We will present the various subsystems involved in imaging snowflakes outside the drone's flow envelope, including synchronizing a pulsed LED circuit to compensate for the large image distance and low numeric aperture. We will present the first snowflakes captured in freefall during the start of the 2024 snow season to demonstrate the feasibility of our airborne microscopy system in hovering flight.

How to cite: Muller, K., Camenzind, M., Shesterikov, I., Morandi, S., and Coletti, F.: Hovering a Microscope on a Drone: Development of UAV Based Systems for High-resolution Imaging of Falling Snow, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17544, https://doi.org/10.5194/egusphere-egu25-17544, 2025.

EGU25-19551 | Posters on site | AS5.8

A multi-gas sensor system lifted by a tethered aerostat for real time in-situ investigation of volcanic plumes 

Salvo Marcuccio, Stefano Corradini, Riccardo Biondi, Francesco Ciancitto, Alessandro Filippeschi, Gaetano Giudice, Matteo Gemignani, Lorenzo Guerrieri, Linda Lambertucci, Irene Marsili, Luca Merucci, Camilo Naranjo, Simona Scollo, and Dario Stelitano

Volcanic eruptions eject a large amount of aerosols and gases in the atmosphere with severe implications on the environment, climate and life on Earth and, in recent times, human society and aviation. Currently, the main technique for observing volcanic clouds relies on remote sensors both from satellites and ground observatories, also using multispectral cameras. However, the composition of volcanic clouds is difficult to assess due to physical limitations of the instruments’ detection capability: satellite and ground based remote sensing systems, generally used to detect and retrieve plume particles and gases, are limited by instrument sensitivity, spatial resolution and uncertainties of particles optical properties and size distribution. Moreover, the presence of high concentration of some gases in the atmosphere (e.g. CO2) makes their estimation impossible inside the volcanic cloud. Therefore, in-situ measurements are necessary to collect ground truth data to validate the remote sensing models and obtain an accurate characterization of a volcanic cloud.

Drone-mounted sensors could compromise the measurements within the plume due to the disturbances caused by the propellers. Additionally, the drone could be contaminated and damaged by the ash. As a less invasive and less expensive alternative, our groups at the Space Systems Laboratory of the University of Pisa together with INGV developed a novel method for in-situ measurements in volcanic clouds: a custom multi-gas sensor package (“Volcanosonde”) lifted by a tethered aerostat inside the plume. A volcanosonde is composed of a set of sensors, integrated on a circuit board, which record the concentrations of the main constituents of a volcanic plume (SO2, HCl, CO2, PM1 – 10) together with the atmospheric parameters (pressure, relative humidity and temperature). In the volcanosonde, data packets are acquired with a frequency of 1 Hz and stored onto an onboard memory, while a timewise subsampled subset of the data is transmitted to a ground station for real-time visualization via LoRa protocol over the 868 MHz ISM band.

We tested the developed apparatus during a measurement campaign in August 2024 on Mt. Etna, Sicily, in the frame of “VOLANDO”, a PRIN project funded by the European Union- Next Generation EU. The system consisted of a sounding balloon including three volcanosondes attached at 50 m intervals on the retaining rope, a stand-alone Optical Particle Counter and a GNSS receiver. The helium-inflated aerostat was raised to 400 m a.g.l. allowing the sondes to enter the plume and make uninterrupted measurements for 3 hours. The experiment was repeated on different days, effectively collecting in-situ data.

The system showed excellent flight behavior and was relatively easy to handle, even in no flat volcanic terrain, allowing for quick re-location of the flying balloon and the attached sondes over several areas of interest. Real time monitoring of the measurements provided the operators with indication of the quality of data collected and guided the right positioning of the flying platform so to achieve an optimal positioning of the volcanosondes within the plume. We estimate that a crew of two with minimal trraining can operate the tethered balloon autonomously under good weather conditions.

How to cite: Marcuccio, S., Corradini, S., Biondi, R., Ciancitto, F., Filippeschi, A., Giudice, G., Gemignani, M., Guerrieri, L., Lambertucci, L., Marsili, I., Merucci, L., Naranjo, C., Scollo, S., and Stelitano, D.: A multi-gas sensor system lifted by a tethered aerostat for real time in-situ investigation of volcanic plumes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19551, https://doi.org/10.5194/egusphere-egu25-19551, 2025.

EGU25-19785 | Posters on site | AS5.8

Greenhouse gas emissions from wastewater treatment plants using drone-based measurements 

Magnus Gålfalk and David Bastviken

Using a drone-based method for simultaneous flux measurements of greenhouse gases (GHGs) we assessed methane (CH4) and nitrous oxide (N2O) at several wastewater treatment plants (WWTPs) with anaerobic digestion.  Results showed unexpectedly high fluxes and discovered that N2O emissions from sludge storage are at least as important as CH4 emissions in terms of global warming. Despite this, N2O emissions from anaerobic digestion sludge are usually assumed to be negligible and therefore not measured routinely at WWTPs. The CO2-equivalent total emissions of CH4 and N2O were 3-fold higher than the IPCC-recommended emission-factor-based estimates. The drone-method works in a wide variety of environments for simultaneous measurements of the major GHG fluxes (CH4, N2O, and CO2) without the need to do repeated flight patterns to cover all gases, alleviating the problem of flux potentially changing between flights which would otherwise make flux comparisons between the different GHGs less reliable.

The drone method used is a further developed version of our previous method (Gålfalk et al 2021 - https://pubs.acs.org/doi/10.1021/acsearthspacechem.1c00106) with longer flight time, higher payload, all major GHGs measured simultaneously, improved logging with all measurements needed for flux calculations being measured on-board the drone without any need for ground-based auxiliary measurements, and more convenient post-processing to calculate fluxes.

How to cite: Gålfalk, M. and Bastviken, D.: Greenhouse gas emissions from wastewater treatment plants using drone-based measurements, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19785, https://doi.org/10.5194/egusphere-egu25-19785, 2025.

EGU25-20658 | Orals | AS5.8

UAV-based measurement of natural gas seeps using a newly developed ultra-lightweight high-sensitivity methane sensor in the western Canadian Arctic 

Jalal Norooz Oliaee, Meghan Beattie, Roger MacLeod, Chase Sun, Joel Corbin, and Peter Morse

Airborne eddy-covariance measurements over the outer Mackenzie River delta in the western Canadian Arctic have linked significant methane (CH4) emissions to geological sources from subsurface reservoirs. However, few natural gas seeps have ever been mapped. Efforts by airborne imaging spectroscopy to locate these methane ‘hotspots’ primarily attributed higher emissions to biogenic CH4 from wetlands as a function of the water table. Resolving the discrepancies between these findings requires identifying seeps within areas of high background emissions. Conducting ground-based measurement surveys to achieve this is challenging in wetlands due to the impedance of widespread bodies of water and the risk of releasing CH4 when disturbing the soil during on-foot surveys.

To aid in identifying methane seeps that have not been mapped before, we present an ultra-lightweight in-situ methane sensor, and its deployment on a common commercially available Uncrewed Aerial Vehicle (UAV) – a DJI Matrice 300 RTK. This system was tested in a location in the Mackenzie River delta where CH4 is known to seep to the surface through conduits in thin, thawing permafrost overlying underground hydrocarbon reservoirs. The easily transportable UAV permits non-invasive, near-surface flight capabilities with highly flexible flight plans, while the sensor’s lightweight and power-efficient design permits high sensitivity for detecting and quantifying subtle variations in atmospheric CH4 concentrations, even in remote and challenging environments.

Our miniaturized, mid-infrared tunable diode laser absorption spectroscopy CH4 sensor targets CH4’s strongest rotational-vibrational transition at the 3270 nm wavelength. Employing the wavelength modulation technique and a small open-path gas absorption cell, the sensor is able to resolve atmospheric CH4 concentrations as low as 10 ppb (parts per billion) with a near-instantaneous response time (100 Hz sample rate) making it suitable for deployment on fast moving aerial platforms. The entire standalone instrument package weighs 1.2 kg and is ideal for integration on consumer UAVs which have limited payload capacities.

We flew the UAV in horizontal grid patterns typically used in source detection and localization scenarios, as well as vertical “curtain” patterns to sample cross sections of the CH4 plume arising from a known gas seep to quantify the flux rate. Preliminary data analysis using a Gaussian plume inversion technique yields a CH4 emission flux estimate near 8 kg hr-1, which is comparable to fugitive emissions from some oil and gas production facilities in Canada. Our results emphasize the significance of this approach to reliably, effectively, and precisely quantify CH4 emission from natural sources, as it will enable us to identify sources of CH4 hotspots and test our hypothesis that the magnitude and frequency of these emissions will increase throughout the study region as the climate warms.

How to cite: Norooz Oliaee, J., Beattie, M., MacLeod, R., Sun, C., Corbin, J., and Morse, P.: UAV-based measurement of natural gas seeps using a newly developed ultra-lightweight high-sensitivity methane sensor in the western Canadian Arctic, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20658, https://doi.org/10.5194/egusphere-egu25-20658, 2025.

EGU25-20826 | Orals | AS5.8 | Highlight

Preliminary results of World Meteorological Organization Uncrewed Aircraft Systems Demonstration Campaign (WMO UAS DC) 

Debbie OSullivan, James Pinto, and Nicolas Rivaben

The WMO Uncrewed Aircraft Systems Demonstration Campaign (UAS-DC) was organised to measure the ability of a range of UAS to meet the requirements for operational upper air observations and to assess their ability to fill observational gaps in WIGOS GBON and/or RBON. Data were collected over a 7-month period from March to September 2024 and 3 Special Observing Periods were performed: during US March 2024 Eclipse, Paris Olympics and during 2024 ISARRA Flight Week Campaign in September, using WMO NetCDF data format standard, which were automatically converted to the BUFR format. These two standardised formats facilitated the widespread use of UAS weather observations by researchers and NWP modelling centres around the world. In addition to deploying a distributed trial network of UAS to test the concept, the campaign used the WMO Information System (Version 2.0, WIS 2.0) to provide real-time data to participating subscribers during the campaign. These highly flexible, accurate and environmentally friendly weather sensing UAS provide a new innovative observing system for National Meteorological and Hydrological Services (NMHSs) to fill observational gaps and subsequently improve numerical weather prediction capabilities. The UAS-DC provided insight into the potential use of crowd-sourced data from observations of opportunity collected by the delivering UAS. We present in this work an overview of the campaign, including a discussion of the methods, and the potential impact that UAS observations collected at regional scales may have, as indicated by initial studies conducted by NWP centres.

How to cite: OSullivan, D., Pinto, J., and Rivaben, N.: Preliminary results of World Meteorological Organization Uncrewed Aircraft Systems Demonstration Campaign (WMO UAS DC), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20826, https://doi.org/10.5194/egusphere-egu25-20826, 2025.

EGU25-28 | ECS | Orals | SM6.1

Mapping Lithospheric Discontinuities and Residual Topography in the Pannonian Basin and Surrounding Orogens 

Dániel Kalmár, Attila Balázs, Laura Petrescu, György Hetényi, Josip Stipčević, István János Kovács, and István Bondár

We perform a comprehensive analysis of P-to-S and S-to-P receiver functions to investigate the lithospheric discontinuities across the Eastern Alps, Pannonian Basin, Carpathians, and Dinarides. The Pannonian Basin, situated in Central Europe, is characterized by thick sedimentary deposits of up to 7 km, resting on a crystalline basement. This basin is enclosed by young orogens, which exhibit thick crust due to prior tectonic activities, such as subduction and collision.
In this study, we provide several new geophysical maps derived from receiver function analysis, including the first detailed maps of sedimentary thickness, Conrad discontinuity, Moho depth, upper and lower crustal thickness, and lithospheric thickness. Our results reveal significant Moho depth variations: from 20-26 km beneath the sedimentary basins to 40-45 km beneath the Eastern Alps and Southern Carpathians. Additionally, we report that the lithosphere is relatively shallow (<90 km) in the Pannonian Basin, while in surrounding orogens, it deepens to 90-140 km, with corresponding variations in surface heat flow values.
Further, we analyse topographic signatures, such as actual, residual, and dynamic topography, to assess the contributions of mantle and crustal processes, as well as surface dynamics. Our findings provide crucial insights into the tectonic evolution and structure of the region, enhancing our understanding of the complex interplay between crustal thinning, lithospheric dynamics, and surface topography.

How to cite: Kalmár, D., Balázs, A., Petrescu, L., Hetényi, G., Stipčević, J., Kovács, I. J., and Bondár, I.: Mapping Lithospheric Discontinuities and Residual Topography in the Pannonian Basin and Surrounding Orogens, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-28, https://doi.org/10.5194/egusphere-egu25-28, 2025.

While extensively studied and well understood in certain regions, the Canadian Shield still presents significant challenges and uncertainties in its northern areas, particularly within the Churchill Province. Two major unresolved aspects in this region are the precise determination of Moho depth and the characterization of anisotropy.

To address these gaps, this study employs DeepRFQC, a state-of-the-art technique for rigorous quality control of receiver function signals. By analyzing all available signals across the area, DeepRFQC ensures that only high-quality data are selected, providing a robust foundation for subsequent analyses.

We used H-k stacking and Harmonic Decomposition to investigate the lithospheric structure. Calculated kappa (κ) values showed strong agreement with gravity data, underscoring the reliability of the results. Harmonic Decomposition revealed anisotropy patterns consistent with the regional stress field, offering new insights into the tectonic processes.

These findings suggest that the observed seismic anisotropy is closely aligned with the region’s predominantly NE-SW geological structures, providing a clearer understanding of the Churchill Province's lithospheric dynamics.

How to cite: Sabermahani, S. and Frederiksen, A.: Understanding the Northern Canadian Shield: Moho Depth, Anisotropy, and Tectonics from Receiver Functions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-495, https://doi.org/10.5194/egusphere-egu25-495, 2025.

Understanding the crustal structure of the Himalayas and the geometry of the underthrusting Indian plate beneath the Himalayan arc provides crucial insights into regional tectonics and enhances earthquake hazard assessment in the region. This study focuses on the Kumaun-Garhwal Himalaya, a region that is proposed as a potential site for a future great earthquake. We obtained the 3D compressional wave (Vp), shear wave (Vs), and P-to-S wave velocity ratio (Vp/Vs) of the region. To achieve this, we employed joint inversion of body wave and surface wave datasets. This integrated approach overcomes the limitations of individual methods, providing a comprehensive view of the crustal structures. The analysis involved inverting the arrival times of 515 local earthquakes recorded at 41 broadband stations spanning the region and also analyzed continuous waveforms recorded by these stations between November 2006 and June 2008. The resulting crustal velocity structure and relocated earthquake hypocenters reveal a flat-ramp-flat geometry of the Main Himalayan Thrust (MHT). Furthermore, the findings offer critical insights into the crustal composition and its role in earthquake generation. These results enhance our understanding of the region's tectonic framework and contribute to better assessment and mitigation of seismic hazards in the Himalayan arc.

Keywords: Seismic tomography; Continental tectonics; Main Himalayan Thrust; crustal imaging.

How to cite: Ali T S, S. and Gupta, S.: 3D crustal structure of Kumaun-Garhwal (central) Himalaya from joint inversion of surface wave and body wave dataset., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-524, https://doi.org/10.5194/egusphere-egu25-524, 2025.

EGU25-586 | ECS | Orals | SM6.1

Seismic imaging of the crustal structure beneath Lebanon and localization of earthquakes 

Ali Janbein, Alexandrine Gesret, Marleine Brax, and Nisrine Makhoul

The Eastern Mediterranean region is characterized by a complex tectonic setting, where the African and Arabian plates converge. This makes Lebanon a seismically active zone that has experienced major destructive earthquakes and could experience similar catastrophic events in the future. Accurate earthquake localization strongly depends on the velocity model used for event location (Gesret et al., 2015). Thus, it is of primary importance to characterize the subsurface structure in order to better locate and understand this seismicity. Characterizing the subsurface crustal structure beneath Lebanon remains challenging due to limited geophysical acquisitions. In this work, we use the P-wave receiver function method to image the subsurface structure beneath two permanent broadband stations, “BHL” and “HWQ”, operational since 2006, which offer a good azimuthal coverage required to characterize dipping interfaces or crustal anisotropy. This study is extended to include several temporary broadband stations distributed across the country to investigate variations in crustal thickness between different regions. Beneath the “BHL” station in western Lebanon, Bayesian inversion of arrival times for PS and PpS phases identifies a Moho boundary at a depth of 33 km, dipping 12° to the southeast. The uncertainties associated to this solution are also estimated thanks to the probabilistic framework. The dip direction aligns with the geological structures of the region. Beneath the “HWQ” station in northern Lebanon, inversion of arrival times and polarities of PS phases from two interfaces suggests an anisotropic lower crustal layer, with a slow axis plunging southwest. This study enabled us to image the crust beneath several broadband permanent and temporary stations and will contribute to the development of a 3D velocity model for Lebanon. In this work, earthquakes are localized using the probabilistic localization method, which will be compared to the deterministic approach commonly used by the National Center of Geophysics in Lebanon. This probabilistic method also provides uncertainty estimates, and allows to compare several velocity models in order to select the best velocity model to be used for event locations in Lebanon.

References

Gesret, A., Desassis, N., Noble, M., Romary, T. & Maisons, C. (2015). Propagation of the velocity model uncertainties to the seismic event location. Geophys. J. Int. (2015) 200, 52–66.

How to cite: Janbein, A., Gesret, A., Brax, M., and Makhoul, N.: Seismic imaging of the crustal structure beneath Lebanon and localization of earthquakes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-586, https://doi.org/10.5194/egusphere-egu25-586, 2025.

EGU25-713 | ECS | Posters on site | SM6.1

Physical and Compositional Characterization of the Greater Alpine Crust Using Seismic Observables 

Henrique Berger Roisenberg, Lapo Boschi, and Fabio Cammarano

The crust, despite being the Earth's outermost layer, remains extremely challenging to study given its heterogeneity and complexities. High-resolution integrated tomographic studies at various scales are essential to indirectly obtain robust information on the compositional and physical properties of the crust. The Greater Alpine Crust (GAC), shaped by the Hercynian, Alpine, and Apennine orogenies, provides a natural laboratory for studying geodynamic processes at plate boundaries. These orogenies have driven the continuous evolution of the European crust from the Paleozoic era to the present day.

This study aims to obtain robust seismic constraints withing the GAC to assess lateral physical and compositional variations. Our approach primarily relies on phase velocity measurements of Rayleigh and Love waves derived from Ambient Noise (AN) tomography, and compressional-to-shear wave velocity ratio (Vp/Vs) and crustal thickness measurements obtained from Receiver Functions (RF). We then use a thermodynamic model, together with independent constraints such as petrology and heat flow data to make interpretations in terms of compositional variation of the crust.

46,041 Rayleigh and 40,028 Love dispersion curves were calculated, and maps of phase velocities were obtained from 3 to 35 seconds. Shear-wave velocity (Vs) maps were derived from surface-wave phase velocity measurements, via a Neighborhood Algorithm. The Molasse, Pannonian, Po, Adriatic, and Tyrrhenian basins are characterized by low Vs (< 2.8 km/s) down to 3 km depth. The Po and Adriatic basins are recognized as low velocity zones down to 10 km depth, with velocities below 3.5 km/s. From 15 km depth the highest velocities of the GAC are in the Tyrrhenian basin (> 4.4 km/s), where the Moho is shallow, while the continental crust presents velocities around 3.5 km/s. From 30 km depth the roots of the Alps, Apennines, Dinarides and Carpathians are clearly visible as relative low velocity zones.

Earthquake data recorded from 2015 to 2023 with a minimum magnitude of 5.5 and a maximum of 8.5, with epicentral distances from 25 to 95 degrees of the center of the study area, were used to calculate P-wave RFs at more than 400 seismic stations using iterative deconvolution. H-κ analysis was performed, using a Moho calculated from AN as a prior. Vp/Vs ratio and crustal thickness were obtained beneath each station. Within our study area, the Moho is deepest under the Alps, Apennines and Dinarides (> 50 km), and shallowest under the Hercynian basement and the sedimentary basins. The lowest Vp/Vs are found in the Moldanubian and Saxo-Thuringian belts (average ~1.70), while the sedimentary basins, and the Alpine and Apennine belts present the largest and most variable Vp/Vs (average ~1.78).

Finally, a comprehensive interpretation of crustal composition and temperature was conducted, integrating constraints from petrological data, heat flux measurements, and thermodynamic modeling. This approach resulted in a new, robust physical and compositional characterization of the GAC.

How to cite: Berger Roisenberg, H., Boschi, L., and Cammarano, F.: Physical and Compositional Characterization of the Greater Alpine Crust Using Seismic Observables, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-713, https://doi.org/10.5194/egusphere-egu25-713, 2025.

EGU25-993 | Posters on site | SM6.1

The topography of the seismic Lithosphere-Asthenosphere Boundary in Iberia and adjacent regions 

Joan Antoni Parera Portell, Flor de Lis Mancilla, José Morales, Xiaohui Yuan, Benjamin Heit, and Jordi Díaz

The lithosphere-asthenosphere boundary, or LAB, is a key element in plate tectonics as it separates the rigid lithosphere from the underlying convecting mantle. Its origin, though, is still not fully understood mainly due to its various definitions (thermal, compositional, etc.), which lead to different LAB depth predictions or measurements. In this study we use more than 34500 S-wave receiver functions to map the depth of the seismic LAB in Iberia and neighbouring regions. We found that the LAB in Iberia is generally shallow, especially along the eastern coast (70 km from the Gulf of Lion to the Alboran Sea) and more locally in the northwest of the peninsula. The LAB only exceeds 90 km depth in the Western Pyrenees and Iberian Range, where there is significant crustal thickening, and also in the Gulf of Cadiz. However, LAB depth and crustal thickness are not always correlated. Most of the major mountain ranges in the region (the Atlas, the Rif, the Betic System and the Pyrenees) feature areas where there is no lithospheric root, with thickened crust (>40 km) underlain by a shallow LAB (<90 km or even <80 km). The LAB depth gradient revealed that this discontinuity changes sharply along the subduction-transform edge propagator (STEP) fault in the Eastern Betics and the area of continental subduction in the Western Pyrenees. Several sublithospheric negative-velocity gradients (NVGs) also occur near these major lithospheric structures, but their origin seems diverse. The most notable NVG is an eastwards-dipping discontinuity under the Strait of Gibraltar, which we identify as the subducted lithosphere of the Gibraltar-Alboran slab. We link additional NVGs below the Alboran Sea to processes related to the slab and the STEP fault, possibly dehydration melting and/or inflow of hotter mantle materials, but the origin of a fourth NVG below the Western Pyrenees and northern Iberian Range is still up in the air.

How to cite: Parera Portell, J. A., Mancilla, F. D. L., Morales, J., Yuan, X., Heit, B., and Díaz, J.: The topography of the seismic Lithosphere-Asthenosphere Boundary in Iberia and adjacent regions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-993, https://doi.org/10.5194/egusphere-egu25-993, 2025.

EGU25-1215 | Orals | SM6.1

Crustal and Upper Mantle Structure Variation Along the Alpine Chain Using Teleseismic Full Waveform Inversion 

Najmieh Mohammadi, Stephen Beller, Vadim Monteiller, and Stephane Operto

The geodynamics of the Alps result from the collision and interaction of the African and Eurasian plates, starting with the closure of the Neo-Tethys Ocean in the Middle Jurassic. This led to subduction, mountain formation, and tectonic shifts, including slab rollback and back-arc basin formation. These processes shaped the complex geological structure of the Alps. Simultaneously investigating the crustal and upper mantle structures is crucial for seismologists to gain a deeper understanding of the geodynamic processes shaping the study region. To reach this aim, we employ Full Waveform Inversion (FWI) on teleseismic earthquakes recorded by AlpArray, SWATH-D, and CIFALPS2 networks to develop the first 3D high-resolution elastic multiparameter FWI model, including Vp , Vs, and density, extending from the surface to 700 km depth. The analysis of FWI models at the crustal scale along the Alps captures small-scale anomalies and velocity variations along fault zones, and reveals the subducted European lithosphere beneath the Adriatic. Our results show that Moho depth increases from the southwestern to the northwestern Alps, with a deeper Moho in the Central Alps compared to the Western Alps. In the Eastern Alps, two distinct Moho structures are identified: the Adriatic Moho, which remains flat at 40 km depth, and the European Moho, which extends southward to 60–65 km and subducts along the Penninic Front. At the upper mantle scale, FWI results show continuous subduction of the European slab beneath the Po Basin to 250 km in the Western Alps, with steeper subduction in the southwest and shallower dips in the north. In the Central Alps, the slab reaches 250 km without detaching, though low-velocity anomalies suggest potential slab tearing. In the Eastern Alps, FWI models indicate vertical slab extension beneath the Tauern window, with a low-velocity anomaly hinting at asthenospheric upwelling due to slab retreat.

How to cite: Mohammadi, N., Beller, S., Monteiller, V., and Operto, S.: Crustal and Upper Mantle Structure Variation Along the Alpine Chain Using Teleseismic Full Waveform Inversion, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1215, https://doi.org/10.5194/egusphere-egu25-1215, 2025.

EGU25-1251 | ECS | Posters on site | SM6.1

Comprehensive Lithospheric Structure of France: Joint Inversion of Seismic, Gravity, and Gradiometry Data 

Farzaneh Dashti, Christel Tiberi, Stéphanie Gautier, and jerome vergne

We present a comprehensive model of lithospheric structure extending to 300 km beneath France, derived from a joint inversion of teleseismic, gravity, and gradiometry datasets. Our analysis incorporates 27,935 relative travel time residuals sourced from the 193 French permanent seismic stations (EPOS-France), alongside 30,351 terrestrial gravity measurements and the complete gravity gradient tensor from GOCE satellite mission. The integration of these three complementary datasets enhances our understanding of lithospheric structures. Our joint inversion method allows for inverting the velocity-density relationship with independent model parametrization.

Through the velocity model, our findings reveal significant lateral variations in P-wave velocity, including a prominent orogen-parallel high-velocity anomaly that extends from the surface to a depth of 135 km, centered beneath the Pyrenees and the Southern Alps. Additionally, we identify a high-velocity body extending from the surface down to 80 km beneath the Massif Central. Notably, our density model highlights several key features, including a narrow high-density body between 10 and 40 km depth, known as the Ivrea body in the Alps. Our results are to compare with previous regional temporary inversions, especially for the northern Pyrenees where velocity and density models are not always coherent. These results contribute to a more nuanced understanding of the lithospheric dynamics in this geologically complex region.

How to cite: Dashti, F., Tiberi, C., Gautier, S., and vergne, J.: Comprehensive Lithospheric Structure of France: Joint Inversion of Seismic, Gravity, and Gradiometry Data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1251, https://doi.org/10.5194/egusphere-egu25-1251, 2025.

EGU25-1672 | Orals | SM6.1

Shaping Western Australia's Geological Framework: Insights from the WA Array Phase One 

Reza Ebrahimi, Ruth Murdie, Huaiyu Yuan, John Paul O'Donnell, Simon Paul Johnson, and Klaus Gessner

In recent years, the deployment of extensive passive seismic arrays across Western Australia has significantly advanced our understanding of lithospheric structures. At the forefront of these efforts is the WA Array program, a transformative 10-year initiative featuring 1,600 broadband stations spanning the entire state of Western Australia. Launched in late 2022, the program has started generating a highly valuable dataset. The data and model outputs from Phase One (from December 2022 to December 2023) mark a long-term effort to compile a state-wide, high-resolution model that will evolve over the course of the program. By integrating this new data with insights from past and ongoing geophysical, geochemical and geological studies, the project aims to unravel the intricate lithospheric structure of the region, ultimately creating detailed models that illuminate Western Australia’s geological history and evolution.
Initial findings reveal significant shallow and crustal features. Measurements of the very shallow subsurface show strong correlation with tectonic setting and also mapped palaeovalleys which have uses in estimation of seismic hazard for engineering projects and potential targets for mineral exploration. Crustal models show significant lateral and vertical variations across geological domains, with the Perth Basin standing out as a prominent low-velocity zone, indicative of basin infill and history of the rifting along the margin of the adjoining craton. The Moho displays flat, distinct transitions in cratonic regions but varies west of the Darling Fault, reflecting the region’s complex tectonic setting. A pervasive NE-SW trend in Moho depth, seismic velocities, and isotopic data suggests compositional segmentation of the Yilgarn Craton into discrete blocks, challenging lateral accretion models and highlighting the influence of deep structures on crustal evolution and resource distribution. Lithospheric imaging further reveals compositional and thermal variations, including deep tectonic features beneath the Yilgarn Craton. An estimate of the lithosphere-asthenosphere boundary exhibits strong spatial correlations between the maximum gradient of the boundary with surface mineralization zones. These observations support the idea that tectonic architecture exerts a fundamental control on resource deposits, consistent with established theories linking deep lithospheric processes to mineral systems. These findings provide valuable insights into the tectonic evolution and resource potential of Western Australia. 

How to cite: Ebrahimi, R., Murdie, R., Yuan, H., O'Donnell, J. P., Johnson, S. P., and Gessner, K.: Shaping Western Australia's Geological Framework: Insights from the WA Array Phase One, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1672, https://doi.org/10.5194/egusphere-egu25-1672, 2025.

EGU25-1878 | Orals | SM6.1

The upper mantle beneath Asia from seismic tomography, with inferences for the mechanisms of tectonics, seismicity, and magmatism 

Yihe Xu, Hui Dou, Sergei Lebedev, Bruna Chagas de Melo, Robert van der Hilst, Baoshan Wang, and Weitao Wang

The structure and dynamics of the upper mantle control tectonics, seismicity, magmatism, and the development of mineral deposits. Seismic tomography maps spatial variations in seismic velocity and offers essential information on the variations of temperature in the mantle, the thickness and mechanical strength of the lithosphere, and the convection patterns below it. Thanks to the growth in the station coverage, tomographic models of Asia reveal increasingly detailed structures.

Here, we present a new waveform tomography model, ASIA2024, constrained by massive global and regional datasets. The data coverage used to construct ASIA2024 is maximised across the hemisphere centred at Asia. In China, in particular, dense national network data enhances the sampling. Our waveform tomography extracts structural information from surface waves and from S and multiple S body waves. The effects of errors are suppressed by statistical and targeted outlier analyses and the removal of the least mutually consistent data.

Extensive comparisons of contemporary tomographic models reveal both consensus features and differences between models and demonstrate relative advantages of different approaches and data types. ASIA2024 advances the resolution of the imaging compared to the state of the art at the scale of the continent. A prominent high-velocity anomaly at lithospheric depths shows the Indian cratonic lithosphere underthrusting and subducting beneath Tibet. In the transition zone below the plateau, a fragmented high-velocity anomaly indicates lithospheric remnants, probably from different phases of subduction. The lithosphere beneath most diamondiferous kimberlites—originally emplaced on thick cratonic lithosphere—is observed to be still thick at present. Relatively low velocities at kimberlite locations are indicative of craton-lithosphere thinning and are detected beneath northwestern Siberian Craton (Siberian Traps) and most of the Indian Shield (Deccan Traps and surroundings), with the exception of the intact cratonic lithosphere beneath northeastern Dharwar Craton. This suggests that the mantle plumes responsible for the traps have eroded the deep cratonic lithosphere.

Thin lithosphere and recent basaltic volcanism are observed in eastern Sino-Korean and Yangtze Cratons, with subduction, stretching, and rifting likely to have weakened and modified their cratonic roots. Cenozoic basalts are found exclusively where the lithosphere is observed to be thin. Beneath the Hainan volcanic region, a low-velocity anomaly is observed throughout the upper mantle, consistent with the previously proposed Hainan Plume feeding the magmatism. The shape of the anomaly indicates a complex morphology of the upwelling. Low-velocity anomalies in the mantle transition zone beneath the Hangai Dome and southern Siberian Craton are consistent with hot upwelling(s) and horizontal asthenospheric flow feeding the dispersed basaltic volcanism.

Sediment-hosted metal deposits tend to be located near contrasts in the thickness of the lithosphere, including craton boundaries and other substantial heterogeneities.

Intraplate seismicity is controlled by plate-boundary stresses and lateral variations of the lithospheric thickness and strength. Areas with relatively thin lithosphere across Asia tend to localise deformation and seismicity. The Gujarat seismic zone in India is collocated with an area of warm, thin lithosphere. This suggests a relationship between the occurrence of devastating earthquakes there and deformation in the mechanically weak part of the plate.

How to cite: Xu, Y., Dou, H., Lebedev, S., Chagas de Melo, B., van der Hilst, R., Wang, B., and Wang, W.: The upper mantle beneath Asia from seismic tomography, with inferences for the mechanisms of tectonics, seismicity, and magmatism, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1878, https://doi.org/10.5194/egusphere-egu25-1878, 2025.

EGU25-1951 * | Orals | SM6.1 | Highlight

Lithospheric structure beneath east Türkiye and implications for the 2023 doublet earthquakes 

Yangfan Deng, Zhou Zhang, Özcan Özyıldırım, Deniz Varilsuha, Xin Li, Umit Avsar, Ahmet Yildiz, Metin Bagci, and Gokhan Kocaoglu

In February 2023, Türkiye suffered two strong earthquakes with a scale of more than 7 Mw, causing serious human and property losses. Previous studies have been conducted close to this area, indicating that lithospheric deformation is mainly controlled by the strong interaction of the surrounding converging plates and is significantly influenced by the distribution of deep fluids. However, due to the sparse observations and resolution of seismic and electromagnetic imaging of subsurface structures, no high-resolution image reveals the relationship between deep structures and strong earthquakes in this region. An international cooperation project is funded to use seismology and electromagnetic data to understand deep structures and processes better. This study aims to apply the newly developed seismic technique to describe the geometry of the key interface in the lithosphere, and newly deployed MT data to reveal the distribution of fluid/partial melt. Constricting the content and spatial distribution of deep fluid, the deformation mechanism, and the fluid behavior of lithosphere under plate interaction will be discussed. The detailed results will be presented in this meeting.

How to cite: Deng, Y., Zhang, Z., Özyıldırım, Ö., Varilsuha, D., Li, X., Avsar, U., Yildiz, A., Bagci, M., and Kocaoglu, G.: Lithospheric structure beneath east Türkiye and implications for the 2023 doublet earthquakes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1951, https://doi.org/10.5194/egusphere-egu25-1951, 2025.

EGU25-2738 | ECS | Posters on site | SM6.1

Anisotropic Anelastic Fresnel-Volume-Migration of the Asse 3D Seismic Data Set 

Niklas Kühne, Felix Hlousek, Stefan Buske, Lena Bräunig, Volker Becker, and Maximilian Scholze

In 2020, a comprehensive 3D reflection seismic survey was conducted over the Asse salt structure in Lower Saxony, Germany, to support the retrieval of radioactive waste from the salt mine. While the data has already been processed using conventional seismic imaging techniques, we present the results from applying the Fresnel-Volume-Migration (FVM) approach that we extended for considering anisotropy and anelastic attenuation. These enhancements aim to provide a more detailed and accurate characterization of the Asse region’s complex geology, which is crucial for the safe planning and execution of the waste retrieval process.

A wavefront construction (WFC) technique was employed to calculate the required Green’s functions for 3D anisotropic (TTI) velocity models. The WFC method was further extended to also calculate compensation traveltime fields (t*) for spatially varying Q-models. These t*-fields were then incorporated into the migration process to account for amplitude decay, phase shifts and dispersion due to anelastic attenuation, ultimately leading to a more accurate representation of subsurface reflectivity.

The method was applied to both synthetic 2D data as well as 3D subsets of the Asse seismic data set. Migration with anelastic compensation effectively corrected amplitude losses and phase distortions in the synthetic data. Furthermore, applying the anisotropic FVM to the 3D Asse data set significantly improved image quality. Additionally, the migration was performed in Common Offset Gather (COG) domain to facilitate muting of the corresponding Common Image Gathers (CIGs) and thereby significantly enhancing the quality of the resulting images.

Our study highlights the critical importance of integrating both anisotropy and anelastic attenuation into 3D seismic imaging to obtain reliable, high-resolution subsurface images. Accurate positioning and characterization of reflectors are essential for performing further quantitative seismic processing, e.g. AVO (Amplitude Versus Offset) analysis, which, in turn, facilitates more precise geological interpretations. The seismic imaging advancements developed here also offer promising applications for other applications, e.g. for mineral exploration, geothermal reservoir characterization, as well as within the radioactive waste disposal site selection process.

How to cite: Kühne, N., Hlousek, F., Buske, S., Bräunig, L., Becker, V., and Scholze, M.: Anisotropic Anelastic Fresnel-Volume-Migration of the Asse 3D Seismic Data Set, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2738, https://doi.org/10.5194/egusphere-egu25-2738, 2025.

EGU25-3499 | Posters on site | SM6.1

Magnetic modeling of the J anomaly and M-series at 31°N, NW Central Atlantic, constrained by crustal structure 

Marta Neres, César Ranero, Manel Prada, Ingo Grevemeyer, and Laura Gómez de la Peña

The high amplitude J magnetic anomaly is usually described as corresponding to the M3-M0 anomalies of the M-series and marks the boundary with the Cretaceous Normal Superchron in the Central Atlantic. A seafloor spreading nature of J is undisputed, but remains debated a potential extension into the southern North Atlantic west of Iberia, with its implications for the kinematic reconstructions of the rift-to-drift transition of Iberia-Newfoundland margins. To image the structure of the J anomaly, coincident wide angle seismic, multichannel seismic and magnetic data were collected across the Mesozoic oceanic crust at ~31°N during the ATLANTIS cruise in 2022. A seismic tomography model reveals a complex velocity structure with significant lateral crustal thickness variation that is at odds with the classical view of a uniformly thick J anomaly crust. Instead of the invoked excess magma production, the structure supports complex variation of the seafloor spreading processes.

We present new magnetic modeling for the ATLANTIS profile that constrains the geometry of the magnetic layers with the seismic velocity model, the basement and Moho topography, and the crustal thickness. We first show the canonical approach of modeling the oceanic crust as a constant thickness layer with alternating polarity blocks, which is not able to match neither the amplitude nor the wavelength of anomalies, either considering constant depth or integrating top of basement topography for the magnetic layer. This may be related to the slow spreading processes that tend to cancel short wavelength anomalies and decrease the anomaly amplitude, which strongly suggests that the crustal structure should be integrated in magnetic modeling, especially of non-fast spreading crust.

We used the seismic velocity structure to constrain the thickness of the magnetic layer, either from 6.0 or 6.5km/s isovelocity contour, or varying proportionally to total crustal thickness. Our results show that the M-series domain (up to M3n) can be modeled by defining the magnetic layer thickness as ~20% of total crustal thickness and with a simplified alternating polarity sequence. For the J-anomaly domain, however, a simple relation doesn’t apply, and adjustments in the layer thickness and magnetization are required. A progressive increase in magnetization is needed from the time of M3n onwards, reaching maximum values between M1r and M0r anomalies and decreasing towards the CNS. The magnetic layer thickness follows the same tendency. However, the crustal thickness varies in a much distinct way: maximum magnetization values are modeled at the thinner crust, and intermediate magnetization is kept for the region where the crust is thicker, already located at the CNS and offset of the highest anomaly amplitude.

These results challenge the use of classical methods to model oceanic magnetic anomalies generated at slow spreading centers, and more particularly, the classical view of the J-anomaly structure. A temporal lag is suggested between the source mantle processes that originated the alteration of magma composition to higher magnetization (mantle fertility / chemical composition) and the increase in crustal thickness (likely more related to mantle temperature).

Work supported by the Portuguese FCT, I.P./MCTES through national funds (PIDDAC): UID/50019/2025, UIDB/50019/2020 (https://doi.org/10.54499/UIDB/50019/2020) and LA/P/0068/2020 (https://doi.org/10.54499/LA/P/0068/2020). 

How to cite: Neres, M., Ranero, C., Prada, M., Grevemeyer, I., and Gómez de la Peña, L.: Magnetic modeling of the J anomaly and M-series at 31°N, NW Central Atlantic, constrained by crustal structure, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3499, https://doi.org/10.5194/egusphere-egu25-3499, 2025.

The imaging of onshore salt-related features remains a persistent challenge in seismic interpretation due to the complex seismic velocity fields and wavefield interactions associated with salt structures. This study explores the feasibility of applying full-waveform inversion (FWI) to a high-resolution onshore seismic dataset acquired for the mapping of potential carbon storage targets within the Gassum region, Denmark, to improve velocity model accuracy and structural characterization of the associated salt dome. The 2D dataset, collected using a dual-element acquisition system combining large-spread nodal and densely-spaced streamer sensors, offers good spatial and azimuthal coverage, making it a suitable candidate for testing advanced inversion techniques.

In this study, we apply FWI using a multi-scale approach to address issues such as cycle skipping and convergence, with initial models derived from ray-based traveltime tomography. By leveraging both low- and high-frequency components of the seismic data and adopting a systematic approach, this feasibility study aims to assess the extent to which FWI can resolve features such as stratigraphic onlaps, fault geometries, and thinning of roof strata above the salt dome. Early results suggest that FWI can enhance the resolution of velocity contrasts and detect velocity inversions, which may lead to improved imaging of previously unmapped features, including shallow and radially divergent faults and sedimentary pinchouts. Furthermore, the integration of FWI with geological data supports the hypothesis of asymmetric dome growth due to uneven loading during its evolution. Challenges such as cultural noise, crooked acquisition geometry, topography variations, parameter sensitivity, and the need for robust initial models remain key considerations.

The study demonstrates the potential of FWI to advance the understanding of salt dome evolution and its implications for geological carbon storage (GCS) in the onshore halokinetic environment. Specifically, the ability to refine structural interpretations and resolve velocity anomalies is helpful for assessing the suitability of halokinetic domes as potential GCS sites. The methodologies tested here can be adapted for use in other salt tectonic settings, offering a pathway for more detailed subsurface characterization in resource exploration and energy transition applications.

How to cite: Westgate, M. and Malehmir, A.: Feasibility of Full-Waveform Inversion for High-Resolution Imaging of Onshore Salt Domes: Case Study from Central Jutland, Denmark, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4050, https://doi.org/10.5194/egusphere-egu25-4050, 2025.

EGU25-4114 | ECS | Posters on site | SM6.1

Rapid Bayesian Seismic Tomography using Graph Mixture Density Networks 

Xin Zhang, Yan Wang, and Haijiang Zhang

A wide range of academic and practical applications require that we interrogate the Earth’s subsurface for answers to scientific questions. A common approach is to image the subsurface properties using data recorded at or above the Earth’s surface, and to interpret those images to address questions of interest. Seismic tomograph is one such method which has been used widely to generate those images. In order to obtain robust and well-justified answers, it is important to assess uncertainties in property estimates.

To solve seismic tomographic problems efficiently, mixture density networks (MDNs) have been used to estimate Bayesian posterior probability density functions (pdfs) which describe the uncertainty of tomographic images. However, the method can only be applied in cases where the number of data is fixed, and consequently cannot be used in a large number of practical applications that have variable sizes of data. To resolve this issue, we introduce graph neural networks (GNNs) to solve seismic tomographic problems. Graphs are data structures that provide flexible representation of complex, variable systems. GNNs are neural networks that manipulate graphs. GNNs can be combined with MDNs (called graph MDNs) to provide estimates of posterior pdfs for graph data. In this study we use graph MDNs to solve seismic tomographic problems by representing seismic travel time data using a graph. We demonstrate the method using both synthetic and real data, and compare the results with those obtained using Monte Carlo sampling methods. The results show that graph MDNs can provide comparable solutions to those obtained using Monte Carlo methods for problems with variable number of data. After training, graph MDNs estimate posterior pdfs in seconds on a typical desktop computer. Hence the method can be used to provide rapid solutions for similar problems with variable sizes of data. We therefore conclude that graph MDNs can be an important tool to solve many practical tomographic problems.

How to cite: Zhang, X., Wang, Y., and Zhang, H.: Rapid Bayesian Seismic Tomography using Graph Mixture Density Networks, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4114, https://doi.org/10.5194/egusphere-egu25-4114, 2025.

EGU25-4219 | Posters on site | SM6.1

Structural Characteristics of Subducting Oceanic Ridges in the Eastern Nankai Trough Region Derived from FWI of OBS Data 

Andrzej Górszczyk, Ryuta Arai, Gou Fujie, Kazuya Shiraishi, Yasuyuki Nakamura, Ayako Nakanishi, and Yanfang Qin

The eastern part of the Nankai Trough is a region of intense tectonic activity where the Philippine Sea Plate subducts beneath the Eurasian Plate. Large interplate earthquakes, such as the Tonankai and Tokai earthquakes, have repeatedly occurred in this area. A notable feature of the region is the paleo-Zenisu Ridge – a ridge subparallel to the trough axis – believed to be subducting beneath the accretionary prism. Previous studies have suggested that the extent of the paleo-Zenisu Ridge is closely linked to the distribution of rupture zones for megathrust and slow earthquakes. However, the precise extent and topography of the paleo-Zenisu Ridge remain poorly constrained.

Within the long-term collaborative project we aim to reconstruct the detailed seismic velocity structure of the eastern Nankai Trough using several dense 2-D wide-angle OBS datasets to better constrain the condition of the paleo-Zenisu Ridge and evaluate its critical role in the region’s tectonic and seismic dynamics. In this study, we apply first-arrival traveltime tomography and time-domain full-waveform inversion to recover high-resolution velocity models along two parallel OBS profiles (spaced ~20 km apart) acquired by JAMSTEC in the eastern Nankai Trough. These profiles integrate OBS data from two legacy seismic dasets (KR07-10_B and KR12-12_Z04; ~4.8 km OBS spacing) with recently acquired coincident profiles (KM23-13), where OBS instruments were deployed between the receiver positions of the legacy surveys. This integration results in datasets consisting of 80 and 97 OBS per profile, with an improved spacing of ~1.6 km.

The dense OBS spacing of the combined datasets enables stable FWI application up to 8 Hz, allowing for detailed reconstruction of the underlying structure of the accretionary wedge and subducting oceanic crust. Our results, combined with other high-resolution velocity models from the Tokai area of the Nankai Trough, reveal variations in the topographic relief of the paleo-Zenisu Ridge along the subduction front axis. These findings suggest a non-uniform impact of the subducting ridge on the overlying wedge, as well as variations in stress distribution, fluid migration, and seismic coupling along the subduction interface. By leveraging additional OBS profiles and advanced inversion techniques, this study enhances our understanding of the paleo-Zenisu Ridge and its role in shaping the tectonic framework of the eastern Nankai Trough.

How to cite: Górszczyk, A., Arai, R., Fujie, G., Shiraishi, K., Nakamura, Y., Nakanishi, A., and Qin, Y.: Structural Characteristics of Subducting Oceanic Ridges in the Eastern Nankai Trough Region Derived from FWI of OBS Data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4219, https://doi.org/10.5194/egusphere-egu25-4219, 2025.

EGU25-4865 | Orals | SM6.1

Lithospheric Thermal Structure and Dynamic Processes of the South China Sea and Adjacent Regions 

Jing Hou, Jian Fang, and Carla Braitenberg

The South China Sea (SCS) and its adjacent regions lie at the junction of the Eurasian, Pacific, and Indian plates, characterized by complex tectonic evolution and diverse lithospheric features. This study integrates magnetic anomaly, gravity, and heat flow data to investigate the lithospheric thermal structure, effective elastic thickness (Te) distribution, and dynamic processes in the region. Curie depth was constrained using EMAG2 magnetic anomaly data with traditional and improved centroid methods, and the lithospheric thermal structure was calculated using the steady-state heat conduction equation. Te was derived from the fan wavelet coherence method based on WGM2012 gravity data, topographic data, and Moho depth models, providing a comprehensive understanding of the thermal and mechanical properties of different tectonic units.

The results reveal that the lithosphere in the SCS basin is thin (40–50 km) with high geothermal gradients and heat flow, resulting in low thermal and mechanical strength and Te values of 10–15 km, indicative of young oceanic lithosphere. In contrast, the northern continental margins exhibit thicker lithosphere (>80 km) with lower heat flow and higher rigidity, reflected in Te values of 25–35 km, which align with craton stability and compressional forces from the Eurasian plate. Transitional crustal regions, such as the Xisha and Nansha Islands, exhibit intermediate lithospheric thickness (50–70 km), geothermal gradients, and Te values (10–20 km), representing a transition between oceanic and continental lithosphere. The subduction zones, such as the Manila Trench, display combined characteristics of lithospheric bending and mantle wedge thermal anomalies, with outer trench regions showing Te values of 15–25 km, while forearc regions exhibit significant weakening with reduced Te.

Dynamic analysis suggests that the diverse lithospheric thermal structure and Te distribution in the SCS reflect the combined effects of seafloor spreading, subduction, and extensional deformation. High temperatures and thin lithosphere in the basin support its extensional setting; low-temperature, high-Te features of continental margins indicate compressional deformation; transitional crust reflects dual controls from continental extension and oceanic spreading; and subduction zones demonstrate complex mechanical interactions, including lithospheric bending, compressional stresses, and mantle upwelling, which significantly impact lithospheric dynamics.

This study provides new insights into the thermomechanical and dynamic evolution of the lithosphere in the SCS and adjacent regions, offering a robust framework for regional tectonic and geophysical research.

How to cite: Hou, J., Fang, J., and Braitenberg, C.: Lithospheric Thermal Structure and Dynamic Processes of the South China Sea and Adjacent Regions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4865, https://doi.org/10.5194/egusphere-egu25-4865, 2025.

EGU25-5692 | ECS | Orals | SM6.1

The 3D Crustal Structure of Wilkes Subglacial Basin and Transantarctic Mountains in East Antarctica - inferred from Joint Inversion of airborne gravity and magnetic data. 

Maximilian Lowe, Tom Jordan, Jörg Ebbing, Max Moorkamp, Chris Green, Mareen Lösing, Teal Riley, and Robert Larter

Heterogeneities in subglacial geology and crustal properties can play a major role in determining the boundary conditions at the crucial interface between the solid earth and the cryosphere in Antarctica. Geothermal heat flow, a parameter closely tied to regional geology, can particularly influence the behaviour of the overriding icesheet. However, direct geological samples which could inform understanding of heat flow and other geological parameters are limited to ice free regions along the coast, high mountain ranges or isolated nunataks, while the origin of geological material transported by glaciers themselves is often ambiguous. Geophysical joint inversion of gravity and magnetic data can therefore play a key role in constraining the geological and crustal properties of the rocks hidden beneath the ice.

We present a 3D crustal model of Wilkes Subglacial Basin and Transantarctic Mountains based on joint inversion of airborne gravity and magnetic data using the “Variation of Information” inversion algorithm incorporated in the software JIF3D. The applied “Variation of Information” technique enforces a coupling in the objective function between inverted susceptibility and density distribution during the inversion. The objective function is minimized iteratively until a reasonable mismatch between observed and inverted data is reached. The coupling ensures that identical geometries in the inverted density and susceptibility distribution are found relating to shared gravity and magnetic sources. This technique provides an enhanced inversion result for interpreting subglacial geology since inverted geometries relate to both petrophysical quantities compared to separately inverting for density and susceptibility distributions.

Our model reveals a large body located in the interior of Wilkes Subglacial Basin interpreted as a batholithic intrusive structure, as well as a linear dense body at the margin of the Terre Adélie Craton. Density and susceptibility relationships of the anomalous bodies, together with their shapes in 3-dimensions are used to inform the composition and the origin of these crustal bodies. Comparing the density and susceptibility values recovered by our inversion with measurements on Antarctic rock samples indicates that the postulated batholitic intrusion is granitic in composition, but distinct from the Granite Harbour Igneous Complex described previously in the Transantarctic Mountains area. Emplacement of such a large volume of intrusive granite can potentially elevate local geothermal heat flow significantly, due to relative concentration of radiogenic heat producing elements such as U, K and Th. Finally, we present a new conceptual tectonic model for the region based on the inversion results, which includes passive margin development ~670 Ma, with the emplacement of the batholith intrusion before the Granite Harbour Suite.

How to cite: Lowe, M., Jordan, T., Ebbing, J., Moorkamp, M., Green, C., Lösing, M., Riley, T., and Larter, R.: The 3D Crustal Structure of Wilkes Subglacial Basin and Transantarctic Mountains in East Antarctica - inferred from Joint Inversion of airborne gravity and magnetic data., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5692, https://doi.org/10.5194/egusphere-egu25-5692, 2025.

EGU25-5885 | Posters on site | SM6.1

Designing a robust seismic full waveform inversion scheme: an extension approach 

Mustapha Benziane, Romain Brossier, and Ludovic Métivier

Full waveform inversion (FWI) has become the standard for high resolution subsurface imaging, in both academia and the industry. FWI is formulated as a data fitting procedure, where the fit between the observed and the synthetic seismograms is improved iteratively. The synthetic seismograms are computed through the numerical solution of a wave equation, they are compared to the observed ones, and the subsurface parameters are updated to improve this fit. This optimization problem is conventionally solved using gradient based optimization strategies, which update a given initial subsurface model iteratively. These optimization approaches often fail to converge to a meaningful solution, when the initial model does not explain the kinematics of the seismic data. That is, the time shift between the observed and synthetic seismograms in the initial model is too large. This is particularly true in active seismic experiments at the crustal scale, where the data lack low frequency content. 

Our strategy relies on modifying the FWI algorithm, in order to help mitigate the ill-posedness of the problem. To do so, we introduce additional parameters to the problem, which help make FWI well behaved. Our strategy makes the receiver position a free parameter, which is included in the optimization. This allows our algorithm to better explain the data kinematically, when the model estimate is poor. Our approach gives rise to a challenging optimization sub-problem, which we solve using stochastic  optimization strategies: namely, Markov-Chain Monte Carlo (MCMC), Simulated annealing methods, and Particle Swarm Optimization (PSO). The latter proved to be a good candidate for our problem. We have also investigated a deterministic optimization strategy, using a dynamic programming approach. This deterministic method is less expensive than the stochastic alternatives. We test our methods using various realistic synthetic cases, obtaining promising results. This has prompted us to extend the method to 3D FWI, and perform synthetic tests, in preparation for a real 3D data application. The preliminary 3D results in synthetic settings are promising. 

How to cite: Benziane, M., Brossier, R., and Métivier, L.: Designing a robust seismic full waveform inversion scheme: an extension approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5885, https://doi.org/10.5194/egusphere-egu25-5885, 2025.

The asthenosphere is commonly defined as an upper mantle zone with low velocities and high attenuation of seismic waves, and high electrical conductivity. These observations are usually explained by the presence of partial melt, or by a sharp contrast in the water content of the upper mantle. Low viscosity asthenosphere is an essential ingredient of functioning plate tectonics. We argue that a substantial component of asthenospheric weakening is dynamic, caused by dislocation creep at the base of tectonic plates. Numerical simulations of subduction show that dynamic weakening scales with the surface velocity both below the subducting and the overriding plate, and that the viscosity decrease reaches up to two orders of magnitude. The resulting scaling law is employed in an apriori estimate of the lateral viscosity variations (LVV) below Earth's oceans. The obtained LVV help in explaining some of the long-standing as well as recent problems in mantle viscosity inversions. This work has been supported by the Czech Science Foundation through project No. 23-06345S

 

Figure 1. Dynamic weakening below Earth’s oceanic plates. Vectors show the absolute plate velocities derived by Müller et al. (2019), obtained with a freely available software package GPlates. Sublithospheric dynamic weakening, w, showed in color, is computed from these velocities using our empirical law, w = 1.5 [1 − exp(−0.3 vP )]. The quantity w represents a first-order estimate of the LVV in the asthenosphere. Grey areas depict Earth’s continents, black and white lines show the major trenches and ridges, respectively (Coffin, 1998).

References:

Patočka, V., Čížková, H., & Pokorný, J. (2024). Dynamic component of the asthenosphere: Lateral viscosity variations due to dislocation creep at the base of oceanic plates. Geophysical Research Letters, 51, e2024GL109116. https://doi.org/10.1029/2024GL109116

Müller, R. D., Zahirovic, S., Williams, S. E., Cannon, J., Seton, M., Bower, D. J., Gurnis, M. (2019). A global plate model including lithospheric deformation
along major rifts and orogens since the triassic. Tectonics, 38 (6), 1884-1907, doi: 10.1029/2018TC005462

Coffin, M. (1998). Present-day plate boundary digital data compilation. University of Texas Institute for geophysics technical report, 174 , 5.

How to cite: Patočka, V., Čížková, H., and Pokorný, J.: Dynamic Component of the Asthenosphere: Lateral Viscosity Variations Due To Dislocation Creep at the Base of Oceanic Plates  , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6882, https://doi.org/10.5194/egusphere-egu25-6882, 2025.

EGU25-7164 | ECS | Posters on site | SM6.1

Uncovering fossil subduction in a mineral-endowed Paleoproterozoic terrain: Reprocessing legacy BABEL seismic lines from Bothnian Bay, Sweden 

Arianna Koufopoulou, Alireza Malehmir, and Magdalena Markovic

In 1989, as part of a collaborative effort involving 12 research institutions and known as the BABEL Project (Baltic and Bothnian Echoes from the Lithosphere), 2,268 km of crustal-scale seismic lines were acquired in the Gulf of Bothnia and the Baltic Sea. The lines were acquired using near-vertical reflection, and wide-angle refraction methods, providing insights into the evolution of plate tectonic processes during the Paleoproterozoic era.

The offshore, near-vertical seismic data were collected using a 3 km-long cable comprising 60 groups of 64 hydrophones, positioned at a depth of 15 m. An airgun array, consisting of six identical subarrays, was used as the seismic source and towed at a depth of 7.5 m. The group spacing, shot interval, and record length varied between the lines. Specifically, in this study, the record lengths for lines 3 and 4 were 25 s, with a group spacing of 50 m and a shot interval of 75 m, while for line 2, the record length was 23 s with a group spacing of 25 m and a shot interval of 62.5 m, respectively. A sampling rate of 4 ms was used for all three lines.

Lines 2, 3, and 4 in the Bothnian Bay are located between the volcanic-hosted massive sulphide belt of Skellefte in Sweden and Vihanti-Pyhäsalmi in Finland. Given the historic value of the data and within the scope of a mineral systems workflow, we have recovered these data digitally to take advantage of modern processing and imaging solutions. Original processing showed divergent reflectivity reaching the lower crust of a Precambrian crystalline basement in the Baltic Shield. In addition, a prominent dipping reflector extending into the upper mantle was imaged, offsetting the Moho by 5-10 km. These findings led to the suggestion, for the first time, of active plate tectonic processes during the Paleoproterozoic time.

The reprocessing work reveals reflections as shallow as 1 s and shows a series of individual reflections and diffraction signals. The Moho boundary is significantly improved in terms of both its signature and trackability and, as in previous investigations, we show a set of sub-Moho reflections dipping down to 23-25 s. Not only have we brought the data to life, but we have also turned them into compelling narratives, providing an enhanced understanding of lithospheric structures in this mineral-endowed region of the world.

Acknowledgments: This work is supported by the Smart Exploration Research Center. The center has received funding from the Swedish Foundation for Strategic Research (SSF) under grant agreement no. CMM22-0003. This is publication SE25-003.

How to cite: Koufopoulou, A., Malehmir, A., and Markovic, M.: Uncovering fossil subduction in a mineral-endowed Paleoproterozoic terrain: Reprocessing legacy BABEL seismic lines from Bothnian Bay, Sweden, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7164, https://doi.org/10.5194/egusphere-egu25-7164, 2025.

Reflection seismics is indispensable for understanding the structural framework of the crust and providing important constraints on mineral system studies. The non-uniqueness inherent in interpreting data from2D crooked seismic profiles acquired over complex geological structures can be reduced by performing 3D reflector orientation analysis (Calvert, 2017), but this requires good azimuthal coverage, which can be enhanced with the deployment of cross-spreads. A new 70-km long reflection seismic profile was acquired across the Palaeoproterozoic Peräpohja belt in northern Finland to shed new light on its structural framework and contribute to development of the new national mineral exploration program. Single-receiver and single-source acquisition was implemented, resulting in excellent data quality. Survey layout was optimized to extract 3D reflector orientations, and included eight additional cross-spreads extending up to 5 km from the survey line spaced every 7-8 km.

3D reflector orientation analysis was performed for both the inline data (i.e. along the main profile) as well as with the cross-spreads included. The main challenge to processing these data is obtaining an optimal refraction statics solution: in the first pass, a combination of 2D inline statics with 2D statics for each cross-spreads was applied. In the second pass, a 3D tomostatics solution was obtained for the complete dataset. The initial results of the reflection orientation analysis suggests that while the additional effort in acquiring the cross-spreads may not be justified for obtaining the structural image (cross-spreads bring more noisy data), orientation attributes (dip and strike) are better resolved, especially at shallower levels, and where gaps in azimuthal coverage are present (i.e. the profile was too straight). With current acquisition capabilities, cross-spreads can be acquired in a cost-effective manner, yet they should be carefully planted to provide reasonable signal-to-noise ratio data, essential for 3D statics and for the orientation analysis itself.

The new seismic data were acquired as a part of the REPower-CEST “Clean Energy System Transition” project, which received funding by the European Union (number 151, P5C1I2, NextGenerationEU).

How to cite: Malinowski, M. and Calvert, A.: A field test of 3D reflection orientation analysis along a 2D crooked line in northern Finland supplemented with additional cross-spreads, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7991, https://doi.org/10.5194/egusphere-egu25-7991, 2025.

EGU25-8651 | ECS | Orals | SM6.1

3D Bayesian Full Waveform Inversion and Efficient Analysis of Prior Hypotheses 

Xuebin Zhao and Andrew Curtis

Spatially 3-dimensional seismic full waveform inversion (3D FWI) is a highly nonlinear and computationally demanding inverse problem that constructs 3D subsurface seismic velocity structures using seismic waveform data. To characterise non-uniqueness in the solutions we demonstrate Bayesian 3D FWI using an efficient variational method called physically structured variational inference to 3D acoustic Bayesian FWI. The results contain the true velocity model, and provide reasonable posterior uncertainty estimates, at a computational cost that is only an order of magnitude greater than that of standard, deterministic FWI. Furthermore, we employ a variational prior replacement methodology to calculate Bayesian solutions corresponding to different classes of prior information, and develop an effective approach to analyse those prior hypotheses by constructing Bayesian L-curves. This provides insight into the sensitivity of the inversion process to different prior assumptions. This opens the possibility that fully probabilistic 3D FWI can be performed at a sufficiently low cost to be practical in small FWI problems, and to be used to test different prior hypotheses.

How to cite: Zhao, X. and Curtis, A.: 3D Bayesian Full Waveform Inversion and Efficient Analysis of Prior Hypotheses, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8651, https://doi.org/10.5194/egusphere-egu25-8651, 2025.

EGU25-8984 | ECS | Orals | SM6.1

A new spatio-temporal misfit function for waveform inversion of DAS data 

Eyal Shimony and Ariel Lellouch

The novel technology of Distributed Acoustic Sensing (DAS) has gained widespread adoption over the last decade and is increasingly applied across various seismic applications. However, its use in Full-Waveform Inversion (FWI) remains limited. A key challenge in utilizing surface DAS data for FWI lies in the heightened sensitivity of DAS-measured strain data to the often highly heterogeneous near-surface compared to traditional inertial measurements. This sensitivity complicates the recovery of the velocity model in deeper regions, which are typically of primary interest.

To address this issue, we propose a new misfit function defined in a time-frequency-location-wavenumber domain, extending the concepts of time-frequency misfits into the spatial domain. By interpreting DAS data as a discrete sampling of a two-dimensional time-space wavefield, rather than a collection of seismograms, we uncover a symmetry between time and space. This symmetry allows us to process the DAS data in both its original domain and the transformed domain in a consistent manner across both domains. The transformation into the time-frequency-location-wavenumber domain is achieved via a two-dimensional Gabor transform, where phase and envelope misfits are defined analogously to their counterparts in the time-frequency domain.

By comparing the sensitivity kernels derived from misfit functions in the time-frequency-location-wavenumber domain with those from the time-frequency domain, we observe a threefold improvement in sensitivity to deeper velocity anomalies relative to near-surface anomalies. This enhancement significantly accelerates, and in high-noise environments enables, the effective use of DAS data in the context of FWI.

How to cite: Shimony, E. and Lellouch, A.: A new spatio-temporal misfit function for waveform inversion of DAS data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8984, https://doi.org/10.5194/egusphere-egu25-8984, 2025.

EGU25-9302 | ECS | Posters on site | SM6.1

Membrane Wave Equation-Based Ambient Noise Adjoint Tomography: Verification and Application 

Zhengyang Li and Yingjie Yang

Traditional ambient noise tomography contains two steps: (1) inverting the 2D phase and/or group velocity maps at different periods based on the dispersion curves of each station pair and (2) point-wise inversion to obtain 1D shear wave velocity model at each grid node and then gather together to obtain a 3D velocity model. In the first step, most studies use the travel-time tomography method based on ray theory or 2D finite-frequency sensitivity kernel that assumes the surface wave travels along the great circle path. This could introduce travel-time biases when surface wave propagates away from the great circle in complex media and further affect the imaging results.

To consider the ray bending effect and the finite-frequency effect simultaneously and to balance the computational efficiency and accuracy, we consider modeling the propagation of surface wave by solving the 2-D membrane wave equation. Sensitivity kernels with respect to phase velocity are constructed using the adjoint method, which could capture significant deviation of the ray path from the great circle path when the velocity perturbation is larger than 20%. Checkerboard tests have been applied to demonstrate the effectiveness of the new tomography method, compared with the finite-frequency tomography method based on analytical solutions. We test our method with ambient noise data in Southern California.

How to cite: Li, Z. and Yang, Y.: Membrane Wave Equation-Based Ambient Noise Adjoint Tomography: Verification and Application, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9302, https://doi.org/10.5194/egusphere-egu25-9302, 2025.

EGU25-9408 | ECS | Posters on site | SM6.1

Reconciling seismic and thermo-chemical models of cratonic lithosphere 

Felix Davison, Sergei Lebedev, Yihe Xu, Sally Gibson, Chiara Civiero, and Javier Fullea

Most published shear-wave (VS) velocity models of cratons include a VS increase with depth below the Moho, with a maximum at 100-150 km depth. This feature is seen in regional and global 3D tomography models and in regional 1D VS profiles. Taken at face value, it implies an oscillatory geotherm, with a ubiquitous temperature decrease below the Moho, which is implausible. The VS increase with depth has thus been attributed to strong compositional layering in the lithosphere. One recent model postulated widespread hydration and metasomatism in the uppermost cratonic mantle, decreasing VS just below the Moho. An alternative model suggested a strong enrichment of the lower cratonic lithosphere in eclogite and diamond, increasing VS but implying an unusual lithospheric composition. Here, we assemble a representative dataset of phase-velocity curves of Rayleigh and Love surface waves for cratons globally, including the all-craton averages, averages over regions in southern Africa, and interstation measurements elsewhere. We perform both thermodynamic and purely seismic inversions and show that the sub-Moho VS increase is not required by the data. Models with equilibrium, conductive lithospheric geotherms and ordinary, depleted-peridotite compositions fit the surface-wave data fully. A model-space mapping quantifies the strong trade-off between seismic velocities just below the Moho and at 100-150 km depth, which is the cause of the ambiguity. The reason why most seismic models contain a VS increase with depth below the Moho is regularization that penalizes deviations from global average reference models, which are much slower than cratonic VS profiles.

How to cite: Davison, F., Lebedev, S., Xu, Y., Gibson, S., Civiero, C., and Fullea, J.: Reconciling seismic and thermo-chemical models of cratonic lithosphere, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9408, https://doi.org/10.5194/egusphere-egu25-9408, 2025.

Imaging of the Moho discontinuity in the trench-outer-rise region of the Japan Trench is a challenging task due to the structural changes that occur in the oceanic crust. This area is shaped by bending-related faults and petit-spot volcanism, which introduce fractures, hydration, and high porosity to the crust. These processes influence seismic velocities and disrupt sedimentary layers. Volcanic activity adds further complexity by creating uneven structures like cracks, dikes, and sills, which weaken seismic signals and make it harder to detect the Moho. These structural changes call for advanced seismic techniques and detailed data to accurately map the crust-mantle boundary.

In this study we examine the structure of the oceanic plate near the Japan Trench, focusing on identifying the Moho discontinuity and related crustal features. Our study relies on a 100-kilometer-long 2D seismic dataset collected by JAMSTEC in 2017. The data were gathered using 40 Ocean-Bottom Seismometers (OBS) placed 2 kilometres apart, capturing wide-angle seismic signals. Such acquisition setting provides a robust framework for analysing the subsurface with the imaging techniques employed in this study.

We employ two imaging techniques that complement each other in addressing the geological complexities of the region. First, we use Reverse Time Migration (RTM) - wavefield-based imaging approach - to produce highly detailed image of discontinuities in the crust and uppermost mantle. RTM was instrumental in identifying the high-resolution Moho and characterizing the variations in the crust-mantle interface. The method allows for handling areas with complex geological structures, such as those affected by bending-related faults and volcanic intrusions, making it an invaluable tool for this study. In addition, we address the challenges of conventional seismic imaging in regions with highly fractured crusts caused by subduction-related bending. To overcome these challenges, we employ the second technique, known as kinematic migration of slope data. The slope represent the horizontal component of the slowness vector at reciprocal receiver position (air-gun shot position) and is calculated as the difference of picked arrival times of the Moho reflection divided by the receiver distance. This approach significantly reduces uncertainties in identifying the Moho discontinuity.

The combination of RTM and kinematic migration proved highly effective in imaging the Moho discontinuity and revealed valuable details about the crust-mantle boundary. By leveraging these complementary techniques, the study successfully overcame the challenges posed by the region's geological complexity. These results demonstrate the importance of high-resolution imaging in advancing our understanding of Earth's interior. The ability to map the Moho with precision not only improves interpretations of subsurface structures but also contributes to broader tectonic and geophysical research. This study underscores the critical role of innovative methodologies in exploring complex geological environments, paving the way for future discoveries.

How to cite: Amirzadeh, Y. and Górszczyk, A.: Reverse Time Migration and Kinematic Migration Approaches for Imaging the Moho in the Outer-Rise Region of the Japan Trench, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9516, https://doi.org/10.5194/egusphere-egu25-9516, 2025.

EGU25-9580 | ECS | Posters on site | SM6.1

Full-waveform Box Tomography for the Lithospheric Structure in South-central Tibetan Plateau 

Qiwen Zhu, Nobuaki Fuji, Cécile Prigent, Satish Singh, and Li Zhao

Tibetan Plateau is resulted from the collision between India and Eurasia ca 55 Ma. The fate of the subducted Indian crust has long been debated. The Hi-CLIMB seismic experiment (Nábělek et al., 2009) presented images indicating that the southern Tibetan Plateau was under-thrusted by the Indian plate up to ~31°N, and the Indian crust was partially decoupled from the mantle below. However, the structure and the dynamics of the underlying mantle remain enigmatic. Various geodynamic models have been proposed to explain the behavior of the mantle lithosphere across this collision zone. These include hypotheses involving lithospheric delamination, rollback, tearing, etc. Further information about the lithospheric mantle beneath Tibetan Plateau is required to better understand the history and current state of this continental collision. In this study, we conduct full-waveform inversion of P-wave and its coda using 14 teleseismic events recorded by the Hi-CLIMB stations, which mainly consist of an 800-km long sub-linear array of 189 broadband seismometers spaced at 5-15 km. Our analyses yield high-resolution 3-D models for the P- and S-wave speeds along with density in the south-central Tibetan Plateau, which covers key geological features including the Genge basin, the Himalayas, and the Lhasa and Qiangtang terranes. Our model resolves P- and S-wave velocity structures from the surface down to ~400 km depth and the density structure in the uppermost 100 km. Our new 3-D multi-parameter model is integrated with results from geochemical and geothermal simulations to evaluate the existing tectonic models, which sheds new light on the state of the Indian lithosphere beneath Tibetan Plateau.

How to cite: Zhu, Q., Fuji, N., Prigent, C., Singh, S., and Zhao, L.: Full-waveform Box Tomography for the Lithospheric Structure in South-central Tibetan Plateau, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9580, https://doi.org/10.5194/egusphere-egu25-9580, 2025.

EGU25-9801 | ECS | Orals | SM6.1

Crustal structure of the Tibetan Plateau and adjacent areas revealed from ambient noise tomography 

Ping Tan, Yun Chen, Xiaofeng Liang, Wei Li, and Chenglong Wu

How the Tibetan Plateau deformed in the Indian-Eurasian continental collision has been long debated, more specifically, over the relationship between the deep processes and surface structural complexity. Here, we use ambient noise tomography to obtain a high-resolution crustal S-wave velocity model beneath the Tibetan Plateau and adjacent areas involving a comprehensive dataset from over 500 stations. Our images reveal that the crustal flow should be in a limited scale according to the intermittent low-velocity zones (LVZs) observed in the middle crust at 20–40-km depth of the Tibetan Plateau. The distributions and strengths of LVZs further imply that different deep processes promote the surface deformation in various regions of the Tibetan Plateau. The LVZs in the northern plateau, collocated potassic magmatism and low velocity anomalies in the upper mantle, should be originated from the lithospheric delamination. However, in the southern plateau, the S-wave velocity showed an apparent lateral segmentation feature correlated with the north-south trending rifts. The feature indicates that the LVZs were likely controlled by the lateral tearing of the subducted Indian mantle lithosphere, which promotes the rifting deformation. Moreover, the LVZ in the central Tibet should have contributed to the formation of the conjugate strike-slip fault system. In the Tarim Basin, our model showed a high-velocity anomaly in the lower crust that may be related to ancient mantle plume activity.

How to cite: Tan, P., Chen, Y., Liang, X., Li, W., and Wu, C.: Crustal structure of the Tibetan Plateau and adjacent areas revealed from ambient noise tomography, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9801, https://doi.org/10.5194/egusphere-egu25-9801, 2025.

EGU25-10504 | Posters on site | SM6.1

Upper mantle shear-wave velocity conversions to temperature and density: open-source V2RhoT_gibbs sheds light into challenges and possibilities 

Judith Bott, Ajay Kumar, Saeid Zarifikoliaee, Tilman May, Ivone Jiménez-Munt, Maria Laura Gomez Dacal, and Magdalena Scheck-Wenderoth

Variations of seismic wave speed, in particular shear-wave velocity (vs), are largely temperature controlled in the Earth’s mantle. Seismic tomography models thus provide us with insights into upper mantle temperature variations, the rheological configuration of the deep lithosphere and, thus, zones susceptible to strain localization within tectonic plates. With this contribution, we introduce V2RhoT_gibbs, an open-source Python tool for converting vs from upper mantle seismic tomography models to temperature and density in a self-consistent thermodynamic manner.

Our conversion approach utilizes an open-source Gibbs-free energy minimization algorithm (Perple_X), which computes the thermodynamically stable phase and mineral assemblages for a given mantle chemical composition (in terms of major oxides of the (Na2O-)CaO-FeO-MgO-Al2O3-SiO2 system) and a wide range of pressures and temperatures. Users of our tool can choose from different thermodynamic databases to constrain the Gibbs-free energy minimization and thus produce lookup tables for upper mantle pressure-temperature conditions and the associated variations in modal composition and simultaneously calculated bulk rock physical properties (e.g., seismic velocities and thermal conductivities). V2RhoT_gibbs is developed to analyze these lookup tables and hence consider the complex, non-linear relations between vs, temperature and mechanical properties. The tool corrects the pre-calculated anharmonic seismic velocities for anelastic attenuation effects and partial melts, and finally allocates thermodynamically consistent values for temperature and density to the vs‑depth-pairs in upper mantle tomographic models.

We will illustrate and discuss the differences between different chemical compositions, representing various degrees of upper mantle depletion, with respect to their effects on the vs-converted temperature and density fields. In addition, we will show V2RhoT_gibbs conversion results to discuss derived depth variations of the thermal lithosphere-asthenosphere boundary for different tectonic settings (convergent and divergent plate boundaries). Finally, we will discuss challenges and possible solution strategies regarding the interpretation of vs variations in the shallowest upper mantle.

How to cite: Bott, J., Kumar, A., Zarifikoliaee, S., May, T., Jiménez-Munt, I., Gomez Dacal, M. L., and Scheck-Wenderoth, M.: Upper mantle shear-wave velocity conversions to temperature and density: open-source V2RhoT_gibbs sheds light into challenges and possibilities, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10504, https://doi.org/10.5194/egusphere-egu25-10504, 2025.

EGU25-11055 | ECS | Orals | SM6.1

Seismic Structure of the Crust and Upper Mantle Beneath SE Tibet Revealed by Ambient Noise Full-Waveform Inversion 

Shi Yao, Yajian Gao, Andreas Rietbrock, Tao Xu, Tingwei Yang, and Han Xiao

The southeastern margin of the Tibetan Plateau has experienced complex tectonic deformation since the Cenozoic collision between the Indian and Eurasian plates. In this study, Empirical Greens’ Functions (EGF) are extracted from the dense ChinArray (phase I) with over 350 broadband stations covering Yunnan and southern part of Sichuan, China. High-quality surface waves are selected from the EGFs and used for the Multi-Scale Time-Frequency Full Waveform Inversion (FWI) to construct a high-resolution crustal and uppermost mantle S-wave velocity model. Our results reveal a high-velocity anomaly extending from the upper crust down to ~100 km depth beneath the inner zone of the Emeishan Large Igneous Province, interpreted as a fossilized magma plumbing system within the lower crust and lithosphere. Additionally, two long low-velocity zones are bounded by major strike-slip faults, with large earthquakes predominantly occurring along these boundaries. The Xiaojiang Fault is first identified as a well-constrained low-velocity zone, cutting through the whole crust, separating the Yangtze and Sichuan-Yunnan high-velocity blocks, while the Red River Fault delineates the boundary between the Yangtze and Indo-China blocks at the lithospheric scale. The eastern boundary of the clockwise crustal material movement beneath the Southeastern Tibetan plateau might be further confined by the Xiaojiang Fault. The strong rotation movement along the Xiaojiang Fault potentially causes the shear heating or partial melting in the crust along the fault, consistent with the distribution of active crust-origin hot springs and high strain rate from GPS observations. In summary, this model shows higher resolution than the previous studies and provides new insights into the crust-lithosphere geodynamic processes and deformation patterns.

How to cite: Yao, S., Gao, Y., Rietbrock, A., Xu, T., Yang, T., and Xiao, H.: Seismic Structure of the Crust and Upper Mantle Beneath SE Tibet Revealed by Ambient Noise Full-Waveform Inversion, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11055, https://doi.org/10.5194/egusphere-egu25-11055, 2025.

EGU25-11678 | Orals | SM6.1

Mapping depletion of continental roots with seismic waves. 

Eric Debayle and Yanick Ricard

High seismic velocity keels extending to depths greater than 200 km underlie the oldest parts of continents, the Precambrian cratons. Although mantle xenoliths suggests that these keels formed early in Earth’s history, the preservation of deep, cold, and highly viscous roots for hundreds of millions of years in a convective mantle remains enigmatic. A classical view is that the excess density due to colder temperatures is compensated for by a light composition that stabilizes high viscosity roots. Here, we map the magnesium number (Mg#, a proxi for mantle depletion) and the Modal content of olivine within cratonic keels, based on the thermochemical interpretation of a global shear velocity model. This thermochemical interpretation requires mineralogical depletion and a decrease of compositional density beneath Precambrian cratons. We observe that depletion is strong above 150 km (Mg#>92), and decreases with depth down to the lithosphere-asthenosphere boundary (LAB). These conditions ensure cratons’s preservation for hundred to billions of years in a convective mantle, in agreement with mantle xenoliths suggesting that high viscous keels formed early in the history of cratons

 

How to cite: Debayle, E. and Ricard, Y.: Mapping depletion of continental roots with seismic waves., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11678, https://doi.org/10.5194/egusphere-egu25-11678, 2025.

EGU25-11926 | ECS | Posters on site | SM6.1

Bayesian tomography-driven inversion of Bouguer gravity: application to the western Alps 

Matteo Scarponi, Thomas Bodin, and Benoit Tauzin

The 3D western alpine lithosphere presents a complex structure and remains subject of active geophysical investigation. In this context, we propose and apply new techniques to combine seismic and gravity data. In particular, we set up a Bayesian inversion of Bouguer gravity anomaly data for the 3D distribution of density at crustal and lithospheric scales. We use the Bouguer gravity anomaly map after  Zahorec et al., (2021) across the western Alps. 

In our setup, we introduce a priori information based on existing seismic tomography models (e.g. Nouibat et al., 2022), to guide the exploration of model geometries for target density distributions. We also use flexible constraints based on known ρ-vS conversion laws (e.g. Brocher, 2005), to define a pool of candidate density models consistent with rock-physics constraints and laboratory observations.

The 3D forward gravity modeling is achieved by discretizing the target volume area into unitary voxels of constant density, accounting for surface topography as well. By pre-computing the gravity effect of each voxel, we significantly decrease the computational cost of forward modeling, thus allowing an exploration of the parameter space with a Monte Carlo sampling approach. In particular, we implement a Markov chain Monte Carlo (McMC) algorithm in a Bayesian framework.
To address the lower resolution power of gravity data, we reduce the dimensionality of the model space by describing volumetric structures with a level-set approach, based on the available seismic tomographic models. This allows to 1) incorporate a priori knowledge of the crustal structure from seismic investigations into the inversion setup and 2) define complex laterally-heterogeneous density structures with a lower number of parameters. While we allow deviations from exact ρ-vS conversion laws, the bayesian framework allows to highlight existing trade-offs among density and geometry, and to tackle the non-uniqueness that often affects gravity data inversions. Finally, this setup allows to benchmark a seismic tomographic model against gravity data while providing a new density model.

We produce a new 3D density model of the western alpine lithosphere, including the Ivrea Geophysical Body at the boundary between the European and Adriatic tectonic plates. Our setup allows us to compare the resolved density values with seismic tomography models locally and with surface geology as well, providing new constraints on subsurface rock structure and composition.

How to cite: Scarponi, M., Bodin, T., and Tauzin, B.: Bayesian tomography-driven inversion of Bouguer gravity: application to the western Alps, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11926, https://doi.org/10.5194/egusphere-egu25-11926, 2025.

The Transantarctic Mountains, a major escarpment separating East and West Antarctica, are of enigmatic origin. The component of their topography which arises due to transient mantle processes (dynamic topography) can be constrained by quantifying and removing the isostatic contribution to topography to define residual elevation. In this way, insight into shaping of the Transantarctic Mountains by mantle processes can be gained. This method is dependent on accurately constraining the thickness and density of the crust and overlying ice in order to sufficiently account for isostatic loading. The TAMNNET seismic network offers an opportunity to study the crustal architecture of the northern Transantarctic Mountains using passive seismic techniques. Autocorrelations of spectrally whitened P-wave coda signals and high frequency (2 - 4 Hz) P-S receiver functions utilise ice sheet reverberations to forward model properties and thicknesses of the ice and subglacial layer. This new method allows for the presence and extent of subglacial sediment to be assessed, characterisation of the subglacial geology and hydrology based on seismic velocities and Vp/Vs ratio, and insight into the temperature of the ice sheet, all of which have important implications for ice sheet dynamics.  Crustal architecture is modelled using lower frequency (0.5 - 2 Hz) receiver functions and empirical relationships between seismic velocity, density and pressure. Using these results to correct for isostatic topography and ice loading yields residual elevations of 1 - 2 km, consistent with the presence of Neogene volcanism in the region, mantle upwellings imaged in tomographic models, and thinned lithosphere identified through rare-earth element modelling of basalts from the Erebus and Hallett Volcanic Provinces. Collectively, these observations imply that dynamic mantle convective processes are integral to the origin and evolution of the northern Transantarctic Mountains, shedding light on the interplay between tectonic processes in the West Antarctic Rift System and the margin of the East Antarctic Craton. 

How to cite: Dunn, A., White, N., and Larter, R.: Passive seismic insights into the subglacial environment, crustal architecture, and dynamic topography of the northern Transantarctic Mountains, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12315, https://doi.org/10.5194/egusphere-egu25-12315, 2025.

EGU25-12952 | Orals | SM6.1

Global SV wave upper mantle model 

stephanie durand, yanick ricard, fabien dubuffet, and eric debayle

We present a summary of all our seismological models based on surface wave observations. First, wen have updated our global SV model that is based on the waveform modelling of more than 3 millions Rayleigh waves recorded since 1976. The tomographic model is built using the same automated scheme as was presented in Debayle et al., GRL 2016, while the number of data has increased by a factor larger than 2. Second, we present new SV wave velocity and radial anisotropy, ξ, global model obtained from the joint inversion of multi-mode Rayleigh and Love wave data. The Rayleigh dataset has been also used in previous studies to constrain the azimuthal anisotropy, the quality factor Q and the melt content. All these models are based on self-consistent datasets and have been obtained with similar regularization and smoothing. All together they confirm that (1) there is no age dependence of the radial anisotropy ξ in the oceanic lithosphere while age is the main parameter controlling Vsv, (2) Positive (ξ > 1) radial anisotropy extends deeper (down to 300 km depth) beneath oceans than beneath continents (3) melt content and azimuthal anisotropy have a significant dependence with age under oceans, particularly under fast plates, (4) cratons appear fast, melt-free and anisotropic, down to 250-300 km depth for the azimuthal anisotropy and down to 150-200 km for the radial anisotropy, a depth coinciding with the detection of a positive velocity gradient, (5) ξ ≤ 1 anomalies are present in the deeper part of the cratonic roots (200-250 km) that could reflect past delamination or compression of the deep lithospheric roots. Out of these observations, we propose a conceptual model that enables reconciling a number of seismic observations. Finally, will present our new online tool (https://fascil.univ-lyon1.fr/) available to explore these tomographic models and to compare with existing ones.

How to cite: durand, S., ricard, Y., dubuffet, F., and debayle, E.: Global SV wave upper mantle model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12952, https://doi.org/10.5194/egusphere-egu25-12952, 2025.

EGU25-13993 | ECS | Orals | SM6.1

Transport-map proposals for efficient MCMC sampling 

Fabrizio Magrini and Malcolm Sambridge

Knowledge of the Earth's interior relies on indirect information collected at or near the surface. Typically, data do not uniquely constrain the subsurface properties and are contaminated by noise, and therefore the solution of ill-posed inverse problems is required. Geophysicists have traditionally addressed such problems through deterministic approaches, seeking a single 'best-fitting' model defined by optimality criteria that reflect our understanding of the problem at hand. In recent decades, Bayesian approaches have become increasingly common, as they characterise the posterior probability distribution of the model conditioned on the observations, thereby quantifying uncertainty.

In this context, Markov chain Monte Carlo (MCMC) methods have emerged as a crucial tool as they allow sampling from posterior distributions of arbitrary complexity. At the core of many MCMC algorithms lies the Metropolis-Hastings scheme. This combines a proposal distribution with a probabilistic acceptance criterion to construct a Markov chain that has the desired target distribution as its stationary distribution. The algorithm is versatile as it rests on mild technical conditions on the proposal, and is thus widely adopted across a broad range of geoscientific inference problems. Yet when the parameter space is large or the forward models are computationally expensive---both common scenarios in geophysical applications---it can become inefficient, resulting in poor chain mixing and slow convergence to the target (posterior) distribution. These challenges underscore the importance of effective proposal mechanisms.

In this presentation, we introduce a novel approach to designing Metropolis-Hastings proposals based on adaptive transport maps. The framework is inspired by recent developments from the field of Applied Mathematics linking Bayesian inference with Optimal Transport theory. The idea is to find a monotone, nonlinear transformation to recast a (complex) target probability distribution into a (simpler) reference distribution that is more amenable to standard MCMC steps. Our key contribution is to parameterise these transformations using invertible neural networks, ensuring monotonicity while gaining the flexibility and expressiveness that neural architectures afford.

The proposed method progresses iteratively. We begin with a standard sampling strategy (e.g., a random-walk Metropolis) to obtain initial draws from the target distribution. These samples inform the training of an invertible neural network that learns to map from the target to a simpler reference distribution, specifically a standard (multivariate) Gaussian. Subsequent proposals are then generated in the reference space, either as global independence moves or local perturbations, and are accepted or rejected following a suitably modified Metropolis-Hastings criterion. As more samples accumulate, the network's parameters are updated, improving overall sampling efficiency. Ultimately, the approach yields not only an ensemble of samples representative of the desired target distribution---just as in standard MCMC---but also a compact, learned representation of it in the network's weights.

We illustrate the proposed paradigm both theoretically and through examples. Preliminary results indicate that transport-map-enhanced MCMC has the potential to significantly accelerate Bayesian sampling across a range of applications.

How to cite: Magrini, F. and Sambridge, M.: Transport-map proposals for efficient MCMC sampling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13993, https://doi.org/10.5194/egusphere-egu25-13993, 2025.

    The Mariana subduction zone, with its relatively simple oceanic subduction structure and water-rich environment, serves as a unique natural laboratory for studying mantle hydration processes and the lithosphere-asthenosphere boundary (LAB). In this study, we analyze passive-source Ocean Bottom Seismometer data from stations deployed across both the forearc and incoming plate regions to investigate the S-wave velocity structure beneath the central Mariana region. By extracting multi-frequency teleseismic receiver functions and surface wave dispersion data, and applying a transdimensional Bayesian joint inversion method that explicitly accounts for water-layer effects, we achieve a high-resolution characterization of the lithospheric subsurface structure. Our findings confirm significant mantle hydration, consistent with previous studies, and reveal a distinct low-velocity zone at the LAB. Unlike conventional passive-seismic studies, which typically describe the LAB as a single sharp velocity reduction, our results indicate a rapid velocity decrease followed by an equally sharp increase, delineating a ~10 km thick melt-rich zone. Our findings highlight the importance of treating the LAB as a complex system rather than a simple boundary, as the melt-rich zone acts as a lubricant, significantly reducing viscosity and facilitating decoupling of the lithosphere from the asthenosphere, thus enabling plate motion.

How to cite: Zhang, J. and Wang, X.: Ponded Melt-Rich Zone at the Base of Lithospheric Plate in Central Mariana Revealed Using Ocean Bottom Seismometer Data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14179, https://doi.org/10.5194/egusphere-egu25-14179, 2025.

EGU25-14243 | Posters on site | SM6.1

Mapping mantle structure of the European plate based on seismic full-waveform inversion methods 

Hao Shen, Kai Tao, and Liang Zhao

The European continent undergoes a series of complicated tectonic processes since the closure of the Tethyan Ocean, including oceanic plate subduction, continental plate subduction, continental collision and orogeny. High resolution 3-D mantle structure under the European plate is key to investigate its geodynamic evolution history. Full waveform seismic inversion for mantle structure has become feasible with the advent of accurate 3D wave propagation codes and the use of adjoint sources to compute the gradient of misfit functions between data and synthetics. The adjoint source, in this approach, depends on how a misfit is defined between data and synthetics. The time or phase shift between data and synthetic has been used in most full waveform inversions for mantle structure. Waves that sample the upper mantle, however, are almost always multi-pathed due to discontinuities, the low velocity zone as well as large amplitude lateral variations, leading to complex waveforms that cannot be fully captured by time/phase shifts. Here we use the normalized correlation coefficient between data and synthetics as a misfit function to simultaneously capture both the phase and relative amplitude information of the waveform, and perform full waveform inversion on a large data set of three component seismic data from Europe. The global 3-D tomography model S362WMANI combined with crustal model EPcrust comprises our starting model. The adopted numerical solver for the wave equation is SPECFEM3D_GLOBAL, a high-accuracy numerical simulation package based on the spectral-element method. We adopt multi-stage inversion method to iteratively enhance the frequency range of the inversion. Our preliminary results show significant improved resolution of the upper mantle structure and provide key constraints on the deep subduction processes of micro-plates in the Europe region.

How to cite: Shen, H., Tao, K., and Zhao, L.: Mapping mantle structure of the European plate based on seismic full-waveform inversion methods, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14243, https://doi.org/10.5194/egusphere-egu25-14243, 2025.

EGU25-14481 | Posters on site | SM6.1

Physics-Informed Neural Networks for multi-frequency surface wave tomography 

Shaobo Yang and Haijiang Zhang

Surface wave tomography based on dispersion is an important approach for resolving the velocity structure of the crust and upper mantle. Traditional surface wave tomography methods based on dispersion data typically require first construction of 2D phase/group velocity maps, followed by a point-wise inversion of dispersion data to derive 1D profiles of shear wave velocity as a function of depth at each grid point, and finally forming the 3D velocity model. However, the 2D tomography method based on ray theory has a strong dependence on the selection of the initial velocity model and regularization parameters. Furthermore, the eikonal tomography method requires dense observations. Therefore, we propose a surface wave tomography method based on a physics-informed neural network, which can construct the phase/group velocity maps of multiple frequencies simultaneously, eliminating the need for repeated separate inversion for each frequency. The network comprises two branches, one branch takes in the coordinates of the virtual source and station as well as period as input to fit the observed surface wave travel times, and the other branch takes in the station coordinates and period to predict the phase/group velocity. The two branches are constrained by the eikonal equation. After the training is completed, the velocity of each grid point in each period can be quarried using the neural network and form the group/phase velpcity maps for each period. We tested the new method using data from the Feidong dense array and the Weifang dense array, and compared the tomography results with those of the traditional method. The test results demonstrate that the new method is a meshless tomography method with data adaptive resolution. In addition, this method does not require an initial velocity model or explicit regularizations. It is highly automatic, simple, and easy to use, with potential to combined with existing dispersion curve automatic extraction methods for automatic tomography without human intervention.

How to cite: Yang, S. and Zhang, H.: Physics-Informed Neural Networks for multi-frequency surface wave tomography, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14481, https://doi.org/10.5194/egusphere-egu25-14481, 2025.

EGU25-14738 | ECS | Posters on site | SM6.1

Lithospheric structure velocity in the Southern Brazilian margin from surface wave analysis 

Carolina Rivadeneyra-Vera, Marcelo Bianchi, and Victor Sacek

Sedimentary basins in the southern Brazilian continental margin have gained special attention in recent years due to hydrocarbon research. Detailed geodynamic models help to understand the basins' evolution, and the choice of the right constraints helps to improve them. However, the oceanic lithosphere structure in this area is poorly investigated by seismological methods, because of the lack of stations. We study the variations in the lithospheric velocity structure along the southern Brazilian passive margin using two types of databases elaborated from the records of 23 stations of the Brazilian Seismographic Network, between 2011 and 2023. The first database is composed of 4781 group velocity dispersion curves generated by 547 teleseismic events of M>5.0 that occurred in the mid-Atlantic ridge and Sandwich Islands, these curves show periods between 15 and 400s, however for higher periods than 100s there are greater uncertainties which makes the dispersion velocities too unstable to be interpreted. The second database contains 226 dispersion curves derived from 30 local events, with magnitudes between 3.0 and 4.0M, that occurred in the offshore region of the Brazilian margin, these curves show periods between 4 and 12 seconds, which sample shallow depths providing important detailed information of the stretched platform region, that can not be sampled by teleseismic data because the absence of short periods.

The regionalization was performed in both databases to identify regional patterns and obtain velocities at different points of interest, between 20 and 40 km are observed velocities with more continental signatures to the south of 20°S, which may be associated with the extension of the continental shelf, while to the north of 20°S are observed higher velocities, indicating a more oceanic lithosphere. Deeper than 40 km, the areas closer to the margin present higher velocities that decrease up to ~100km depth, as far as we have an acceptable resolution. We also observe less strong velocity anomalies with depth, reflecting a more homogeneous lithosphere. Close to 20ºS latitude is observed a negative anomaly for depths greater than 40 km, suggesting a correlation with Trindade's plume. The regionalized curves extracted in points closest to the platform are consistent with PREM continental velocities up to 30 km, while depths between 30 and 70 km present higher velocities than PREM reference model. Previous studies also found similar velocity patterns in the continental margin; however, these do not present results at shallower depths, such as close to the bottom of the crust and the top of the mantle lithosphere.

The regionalization of the local database gives us essential information up to 10km depth, where important basins and the pre-salt region are located. Despite the low quantity of curves, it is possible to observe a clear positive velocity anomaly at 5km depth, that matches with the pre-salt limits as well as with the Brazilian offshore seismicity. The final 1D inverted velocity models will be interpreted and linked with existing geological and geophysical information to improve the knowledge of the basins in the Brazilian margin.

How to cite: Rivadeneyra-Vera, C., Bianchi, M., and Sacek, V.: Lithospheric structure velocity in the Southern Brazilian margin from surface wave analysis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14738, https://doi.org/10.5194/egusphere-egu25-14738, 2025.

EGU25-15334 | ECS | Posters on site | SM6.1

Ongoing craton destruction driven by pre-existing structures in the central North China Craton 

Cong Ji, Zhouchuan Huang, and Götz Bokelmann

It is significant to constrain the anisotropic crustal and lithospheric structures of the North China Craton (NCC) to understand the mechanisms of craton destruction. The NCC consists of the cratonic Ordos block, the Shanxi Rift, and the severely destructed eastern NCC. The Datong volcano zone (DVZ), which is located in the northern Shanxi Rift, suggests active magmatism and volcanism during the Cenozoic. In contrast, the magma-poor southern Shanxi Rift poses a significant challenge in demonstrating the rifting mechanism and processes. Using the database from ChinArray, we obtain anisotropic Rayleigh-wave phase velocity maps by Eikonal tomography and further invert for the 3-D S-wave structure and its azimuthal anisotropy. Strong azimuthal anisotropy with fast polarization directions parallel to the edge of the low-velocity zone is revealed at a depth of 50~60 km to the west of the DVZ, which is the uppermost mantle near Moho. Our results suggest that the magmatic underplating transfers horizontally in the northern NCC and causes ongoing craton destruction by thermal and chemical erosion. We propose that the subduction of the Paleo-Asian Ocean during the Mesozoic, which is a pre-existing structure, may have contributed to lithospheric activation and localized lithospheric thinning in the northern NCC and results in the north-south differential lithospheric deformation. Similar to the Shanxi Rift, other rift systems, such as the Baikal Rift and the Eastern African Rift, may also be the consequence of the lateral motion of an adjacent cratonic block on its margins. The presence of magmatism within the rift zone is mainly dependent on pre-existing structures, such as subduction.

How to cite: Ji, C., Huang, Z., and Bokelmann, G.: Ongoing craton destruction driven by pre-existing structures in the central North China Craton, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15334, https://doi.org/10.5194/egusphere-egu25-15334, 2025.

EGU25-16082 | ECS | Posters on site | SM6.1

Unraveling the Adriatic Plate Configuration beneath Albania with Teleseismic Full Waveform Inversion 

Yajian Gao, Andreas Rietbrock, Michael Frietsch, Hans Agurto-Detzel, Sofia Kufner, Edmond Dushi, Besian Rama, Damiano Koxhaj, Frederik Tilmann, Bernd Schurr, Xiaohui Yuan, Benjamin Heit, and Bin He

The eastern margin of the Adriatic plate stands out for its tectonic complexity and geohazard potential in Europe, which are dominated by the northeast-directed subduction and collision of the Adriatic plate with the Eurasian plate beneath the Balkan. Beneath the southern Dinarides (northern Albania), the Adriatic plate is believed to be shallower than 150 km whereas the plate penetrates down to 200 km depth beneath the northern Hellenides (central and southern Albania). Further south, the Kefalonia transform fault system (KTFS, northwestern Greece) is believed to represent the transition from continental subduction of Adriatic plate to the oceanic subduction of the Ionian plate. Recent studies proposed different conception models including horizontal and vertical slab tearing beneath these transitions. Despite the importance of this region, seismic imaging is still insufficient to resolve these fundamental geodynamic processes.

To answer these important geodynamic questions, we employ the advanced wavefield-injection teleseismic full waveform inversion (TELEFWI) to image the seismic velocity structure beneath Albania. The TELEFWI explores waveform recordings from 9 high-quality teleseismic earthquakes recorded by 50 broadband stations from the ANTICS array (Albanian Tectonics of Continental Subduction, FDSN code X3, 2022-2024). TELEFWI reveals detailed structures from the crust down to 220 km in depth, with spatial resolution of 20 km for the P wave velocity from crust down to the upper mantle and 15 km for the S wave in the crust and uppermost mantle.

The new velocity model displays a strong eastward-dipping high-velocity anomaly in the upper mantle down to at least 150 km for the whole study domain, which we suggest to be the expression of the subducting Adriatic plate. The Adriatic plate displays westward-retreating pattern in the upper mantle to the coast beneath southern Albania. Meanwhile, multiple high velocity anomalies in depth probably indicates multi-phase slab break-off events at depths of 100 to 150 km beneath southern Albania. In contrast, the Adriatic plate remains relatively flat for over 100 km from the coast to the inland and then dips into the upper mantle beneath northern Albania, but the anomaly is relatively weaker compared to the south. Strong low-velocity anomalies in the upper crust are observed beneath the basins, probably representing the thick sediment layer.

In summary, this study provides a high-resolution velocity model for the first time based on teleseismic full waveform inversion and sheds light on the Adriatic plate configuration beneath its eastern margin.

How to cite: Gao, Y., Rietbrock, A., Frietsch, M., Agurto-Detzel, H., Kufner, S., Dushi, E., Rama, B., Koxhaj, D., Tilmann, F., Schurr, B., Yuan, X., Heit, B., and He, B.: Unraveling the Adriatic Plate Configuration beneath Albania with Teleseismic Full Waveform Inversion, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16082, https://doi.org/10.5194/egusphere-egu25-16082, 2025.

EGU25-16712 | ECS | Posters on site | SM6.1

Glacier structure and icequakes characterization at Argentière using elastic full waveform inversion 

Arthur Grange, Romain Brossier, Ludovic Métivier, and Philippe Roux

Glaciers, which store nearly 70% of the Earth's freshwater, are undergoing significant changes due to accelerating melting caused by climate change. A better understanding of their behavior and mechanisms is therefore crucial for the years to come. To study these processes, a dense seismic array was deployed on the Argentière Glacier in the Mont Blanc massif (French Alps). The sensor array consists in 98 3-component seismic stations which continuously recorded surface displacements over 35 days in early spring 2018. This period coincided with rising temperatures and rapid glacier evolution, so the sensors captured thousands of events, mostly icequakes.

The aim of this study is to reconstruct the glacier's structure and study icequake mechanisms using elastic Full Waveform Inversion (FWI) on the 3-component data. As the data come from a passive seismic experiment, we have no information about the sources. Before reconstructing the structure it is therefore necessary to work on source parameters estimation. These parameters include spatial localization and mechanism. 

First, we detect and localize the icequakes inside the glacier using a beamforming method called Matched Field Processing (MFP). The detected icequakes are observed to be located mostly at the positions of crevasses on the glacier's surface. Then, we decompose the icequake mechanism into a moment tensor and a time signature wavelet. To estimate these two parameters, we develop a joint inversion method based on waveform analysis using an iterative alternating minimization algorithm. The type of mechanism and the source orientation are then interpreted through the eigenvalue and eigenvector decomposition of the estimated moment tensor. The Fundamental Lune representation is employed to statistically study the distribution of more than 14,000 icequake mechanisms within the glacier, revealing a significant proportion of opening and closing mechanisms associated with crevasses. In certain areas, Double-Couple (DC) mechanisms can also be observed, potentially corresponding to crevasse fault slip events.

Using the estimated source parameters, FWI can be applied to reconstruct the glacier structure. A 3D synthetic crevasse model was created to mimic reality, incorporating the three observed crevasse clusters on the glacier, to evaluate the effectiveness of FWI in reconstructing the model in a given frequency-band. The parameters used in the model include S-wave and P-wave velocities, as well as density. The inversion results reveal several key findings: first, multi-parameter inversion with both S-wave velocity and density yields better results. Second, crevasses can be accurately reconstructed within the considered frequency band, provided the source parameters are well-estimated. Finally, the accuracy of source mechanism estimation significantly impacts the quality of crevasse reconstruction. Importantly, iterating between mechanism estimation and structure reconstruction yields improved results, providing promising insights.

How to cite: Grange, A., Brossier, R., Métivier, L., and Roux, P.: Glacier structure and icequakes characterization at Argentière using elastic full waveform inversion, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16712, https://doi.org/10.5194/egusphere-egu25-16712, 2025.

EGU25-16767 | Posters on site | SM6.1

Seismic ambient noise imaging of Xinfengjiang reservoir and adjacent areas, Guangdong, China 

Zuoyong Lyu, Xiuwei Ye, and Genggeng Wen

The Xinfengjiang Water Reservoir (XWR) in the northwest of Heyuan city, Guangdong province, China, has hosted a large number of earthquakes since its impoundment. It is one of the reservoirs that have experienced earthquakes of magnitudes greater than 6, making it one of the most active seismic zones in Guangdong. After the significant increase in seismic activity since the reservoir water storage, many researchers have conducted a series of geophysical studies in the area. However, because of the station coverage restrictions, the detailed seismic structures within XWR have not been resolved, and the understanding of its seismic mechanism and future earthquake disaster risk are still unclear. In this study, we construct a high-resolution shear-wave velocity model in the whole crust at depths from the surface to ∼30 km based on both permanent and temporary stations deployed surrounding the XWR using ambient noise tomography. The permanent stations belong to the Guangdong Earthquake Early Warning Network, including stations equipped with broadband velocity instruments and stations equipped with acceleration strong motion instruments. The temporary stations belong to a short-period seismic array deployed surrounding the XWR in 2023, with a continuous recording duration of 30 days. The imaging results above 5 km show that, with the Heyuan-Shaowu Fault as the boundary, the XWR shows a high-speed anomaly and the Heyuan Basin shows a low-speed anomaly. We also found significant low wave velocity anomalies below the XWR at depths of 5-15 km. Although we have only obtained preliminary velocity models at the crustal scale in the area and made some discoveries, it can still promote a deeper understanding of the crustal structural characteristics and seismic mechanisms of the XWR and its adjacent areas.

References

Ye, X. W., Deng, Z. H., Huang, Y. M., Liu, J.-P., Wang, X.-N., Liu, J., & Tan, Z.-G. (2017). The characteristics of 3D P-wave velocity structure of Middle-upper crust and reservoir water infiltration-diffusion in Xinfengjiang Reservoir of Guangdong. Chinese Journal of Geophysics, 60(9), 3432–3444.

He, L., Sun, X., Yang, H., Qin, J., Shen, Y., & Ye, X. (2018). Upper crustal structure and earthquake mechanism in the Xinfengjiang Water Reservoir, Guangdong, China. Journal of Geophysical Research: Solid Earth, 123, 3799–3813.

Dong, S., Li, L., Zhao, L., Shen, X., Wang, W., Huang, H., et al. (2022). Seismic evidence for fluid-driven pore pressure increase and its links with induced seismicity in the Xinfengjiang Reservoir, South China. Journal of Geophysical Research: Solid Earth, 127, e2021JB023548.

How to cite: Lyu, Z., Ye, X., and Wen, G.: Seismic ambient noise imaging of Xinfengjiang reservoir and adjacent areas, Guangdong, China, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16767, https://doi.org/10.5194/egusphere-egu25-16767, 2025.

EGU25-16907 | ECS | Posters on site | SM6.1

Seismic Imaging from scattered waves using  Distributed Acoustic Sensing offshore Central Chile 

Clara Vernet, Diane Rivet, Alister Trabattoni, and Marie Baillet

Distributed Acoustic Sensing (DAS) is becoming a standard solution for ocean-bottom seismological acquisition by providing a dense and long-distance measurement of ground deformation along offshore submarine fiber-optic cables. In the context of an offshore deployment in Central Chile, fiber-optic cables provide real-time seismic data dominated by scattered and converted phases. In a previous work, we have developed a methodology to determine both the velocity and thickness of the shallow sedimentary layer under the fiber using surface waves and split P-waves. Our current objective is to enhance the crustal imaging by identifying fault zones characterized by strong wavefront scattering and sharp lateral velocity contrasts, and sedimentary basins geometry at sub-kilometer scales in the same area, using scattered surface waves.

We focus on seismic events recorded along a 150-km-long fiber in Central Chile. After partitioning the wavefield to separate direct waves from surface waves, we compute local backprojections of the scattered wavefield. By analyzing multiple seismic events across different frequencies, we investigate variations in wave propagation at multiple scales. The resulting energy profiles reveal spatially resolved fault zone structures and sharp lateral contrasts that align with topographic and structural features. Additionally, using standard seismic noise processing procedures, we compute time-domain cross-correlation functions, autocorrelations, and spectral densities. These analyses provide further insights into the behavior of surface waves near reflector features. For instance, we identify lateral discontinuities associated with basin edges by measuring their frequency-dependent resonance.

Finally, to assess the seismogenic potential of the imaged structures, we will compare the geographical distribution and extent of the detected structures with the shallow seismicity automatically detected in the area using DAS data.

How to cite: Vernet, C., Rivet, D., Trabattoni, A., and Baillet, M.: Seismic Imaging from scattered waves using  Distributed Acoustic Sensing offshore Central Chile, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16907, https://doi.org/10.5194/egusphere-egu25-16907, 2025.

EGU25-17666 | ECS | Posters on site | SM6.1

High-resolution SH-wave crosshole seismic full-waveform inversion in the glacially overdeepened Tannwald Basin 

Sarah Beraus, Daniel Köhn, Thomas Burschil, Hermann Buness, Thomas Bohlen, and Gerald Gabriel

During the Quaternary, the Rhine Glacier formed several overdeepened valleys, including the Tannwald Basin (ICDP site 5068_1, Germany) about 45 km North of Lake Constance. These structures form sedimentary climate archives and thus help to understand climate dynamics in the Alps.

To obtain very high-resolution images of the sediment, seismic crosshole data was acquired using a high-frequency borehole source that predominantly generates SH-waves. The source was excited very meter at 78 to 143 m depth, and the wavefield was recorded at a depth of 105 to 134 m using an eight-station three-component geophone string in a second borehole 28 m away. Given the receivers are spaced 2 m apart along the receiver string, it was moved by 1 m after shooting at all positions. The orientation of both the source and the receivers was done manually, though a calibrated compass attached to the receiver string facilitated this procedure, in constrast to the source orientation.

The SH-data is characterized by a high level of complexity, despite the lithology from a core obtained from one of the boreholes suggesting a predominantly homogeneous material, i.e., fine glaciolacustrine sediments. Additionally, the high-frequency, large-amplitude, long-coda P-wave masks the SH-wave arrivals.

In preparation for full-waveform inversion (FWI), we mute the trigger peak at time zero, perform data reorientation to account for misaligned sources and receivers, apply a 3D-to-2D spreading correction, delay the wavefield by 0.1 s to ensure convergence of the source-time-function inversion, and normalize the data shot-wise. In a previous study, we derived a traveltime tomography model from an additionally acquired SV-wave dataset, which we use as a starting model.

We apply 2D elastic mono-parameter (vSH) time-domain FWI using the finite-difference method to invert the transverse component data. To mitigate the non-linearity of the problem, we use the multi-stage approach with frequencies starting at 100 Hz. To reduce the effects of source and receiver coupling, the global correlation norm is chosen as the misfit function. The misfit is minimized iteratively by means of an optimization through the quasi-Newton l-BFGS algorithm, which reduces the memory requirements and provides faster convergence. Furthermore, to reduce short-wavelength artifacts, the gradients are smoothed with a Gaussian filter. Source-time-function inversion is performed by a stabilized Wiener deconvolution in the frequency-domain using the Newton method with Marquardt-Levenberg regularization. Additionally, we apply frequency-adaptive time-windowing to precondition the data.

Despite the limited parameter space in the isotropic SH-case, the FWI does not yield convincing results. In this study, we explore the potential factors contributing to this outcome, including the data quality and properties, as well as our FWI approach.

 

How to cite: Beraus, S., Köhn, D., Burschil, T., Buness, H., Bohlen, T., and Gabriel, G.: High-resolution SH-wave crosshole seismic full-waveform inversion in the glacially overdeepened Tannwald Basin, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17666, https://doi.org/10.5194/egusphere-egu25-17666, 2025.

EGU25-17757 | ECS | Orals | SM6.1

Joint inversion of surface dispersion and P-wave tomography for temperature and lithology: Methodology and case study in the Eastern Alps  

Stefan Mroczek, Frederik Tilmann, Sascha Zertani, Timm John, Emanuel Kästle, and Kuan-Yu Ke

Seismic observations are usually inverted for seismic velocity structure (Vp and Vs). By using Markov-chain Monte Carlo (McMC) inversion (i.e. solving the forward model and comparing it to the data many times and exploring the virtual space of possible solutions), it is possible to directly invert for rock type as a categorical variable (rather than its constituent minerals and parameters). McMC also manages any non-linear relationships that rock constituents and parameters may have with velocity that could result in non-convergence of a linear inversion. 

We have developed a theoretical and software framework to perform an inversion of surface wave dispersion and P-wave tomography directly to crustal rock type and, by fixing surface and lithosphere-asthenosphere boundary temperature, temperature gradient. 

This approach constrains the inversion to petrologically valid models rather than the larger space of seismologically valid models. Additionally, knowledge of rock type helps to facilitate interpretation by inferring, from the seismic observations, the various lithologies in an unbiased manner. In the crust, the forward model for inferring Vp, Vs, and density from rock type is slow. To overcome this, we calculate a look-up table of seismic properties for crustal rocks as a function of pressure and temperature. 

We demonstrate the method with a synthetic test that shows that velocity and the silica content (mafic-felsic) of crustal layers can be reliably recovered as well as some indication of the main constituent minerals. Temperature and exact mineral assemblage are poorly constrained. A test transect of seven stations in the Eastern Alps indicate a mainly felsic upper crust with a more intermediate lower crust. Temperature, although not well constrained, shows an increase where historic magmatic activity between two major tectonic faults has been previously inferred.

How to cite: Mroczek, S., Tilmann, F., Zertani, S., John, T., Kästle, E., and Ke, K.-Y.: Joint inversion of surface dispersion and P-wave tomography for temperature and lithology: Methodology and case study in the Eastern Alps , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17757, https://doi.org/10.5194/egusphere-egu25-17757, 2025.

EGU25-19393 | ECS | Orals | SM6.1

Quantifying fault-related uncertainty with inverse homogenization 

Giusi Ruggiero, Paul Cupillard, and Guillaume Caumon

Although the ease and accuracy of seismic interpretation are continually increasing thanks to the increasing amount of available data, computing power and new automatic interpretation techniques, it is still challenging to resolve fine-scale geological features at depth (e.g. faults) because of physical limitations. Indeed, seismic imaging techniques are based on frequency band-limited seismic data, and therefore they can only recover a smooth version of the true Earth, which is not suited for a proper geological interpretation below the decametric scale. Uncertainties and pitfalls in the interpretation of these fine-scale features can affect natural hazard mitigation strategies, and lead to overly optimistic model-based forecasts. To make sure that such subtle features are appropriately considered in subsurface uncertainty studies, we propose the use of a downscaling (or inverse homogenization) approach.

In this work, the downscaling is used to properly detect faults and quantify the uncertainty associated to fault parameters geometry and displacement. In particular, from a smooth representation of the real complex structures, obtained through seismic techniques, such as the well-known Full Waveform Inversion (FWI), the downscaling inversion aims to recover all the finer scale fault models compatible with the FWI solution. Because this is an ill-posed inverse problem, the inversion is cast into a Bayesian framework, which combines the information at larger scale coming from the data (FWI model) with some a priori knowledge on the fault structures in order to retrieve a probability distribution over the possible fine-scale models. A Markov Chain Monte Carlo (MCMC) algorithm is adopted to sample the model space and numerically evaluate the posterior probability distribution. This involves the stochastic generation of velocity model realizations where fault displacement is computed using a kinematic modeling approach and the fine-layering velocity is obtained through geostatistical simulations.

A significant advantage of this technique is that it can be applied to downscale a localized area of interest within a larger FWI dataset, consequently reducing memory consumption and computational cost. This latter is also reduced thanks to the inexpensive forward modeling operator (i.e., the non-periodic homogenization), making the stochastic inversion feasible compared to standard MCMC-based seismic inversion methods. The proposed methodology, validated on a synthetic data-case example, proves to be a reliable approach to resolve and quantify fault-related uncertainty.

How to cite: Ruggiero, G., Cupillard, P., and Caumon, G.: Quantifying fault-related uncertainty with inverse homogenization, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19393, https://doi.org/10.5194/egusphere-egu25-19393, 2025.

EGU25-21263 | ECS | Posters on site | SM6.1

Enhanced Subsurface Imaging of Western Nankai Trough Using Full Waveform Inversion 

Anu Yadav, Andrzej Górszczyk, and Rafael Almeida

The Nankai Trough, where the Philippine Sea Plate converges beneath the Eurasian Plate, is situated off SW Japan and is one of the most seismically active subduction zones in the world, producing earthquakes such as the 1944 Tonankai and 1946 Nankai events. Within the Nankai Trough, the region of Shikoku is a geologically distinct segment located within the Tonankai and Nankai rupture zones. Shikoku is distinct due to the presence of a geological backstop, where the rigid forearc crust of the Eurasian Plate resists deformation, causing the compression and thickening of the accretionary prism. This backstop effect creates a structural boundary that influences sediment accretion, tectonic stress distribution, and seismic rupture behavior. The subducting Shikoku Basin crust is thinner and has a shallower dip angle in comparison to the other parts of the trench. The shallow subduction angle beneath Shikoku leads to highly heterogeneous stress and deformation patterns in the accretionary prism compared to steeper-dipping segments. Previous studies employing wide-angle seismic reflection and refraction surveys and tomographic methods have provided valuable insights into the broad-scale structure of the region. These efforts have delineated the geometry of the subducting Philippine Sea Plate and regional velocity structures within the accretionary prism and forearc. However, conventional methods often fail to resolve heterogeneities and variations in the deep subduction interface that critically influence seismic coupling. Furthermore, the role of Shikoku’s unique backstop configuration and the characteristics of the subduction interface at depths exceeding 40 km remain poorly constrained due to the limited resolution of traditional imaging techniques.

To overcome this, we take advantage of wide-angle data from ocean-bottom seismometers (OBS) spaced at 5 km along seismic profiles SK01, SK02, and SK03, acquired between 2009–2010 by the Japan Agency for Marine-Earth Science and Technology (JAMSTEC). We carry out Full Waveform Inversion (FWI) of the OBS data, a cutting-edge seismic imaging method leveraging the complete seismic waveform data to produce high-resolution velocity models of the subsurface. FWI iteratively refines the velocity model by minimizing discrepancies between observed and simulated seismic waveforms, enabling higher resolution at greater depths with unprecedented accuracy.

The obtained high-resolution velocity models provide a clear representation of previously under-resolved features in the off-Shikoku region, particularly the crustal structure and geometry of the Moho. These models overcome the limitations of traditional methods in imaging the subsurface at greater depths, addressing critical gaps in geological interpretation and advancing our understanding of tectonic processes in the region. By revealing fine-scale details of the subducting crust and Moho, this study further aids in developing effective planning for megaquakes and tsunami risk strategies and provides insights that could be applied to other regions with similar tectonic characteristics.

How to cite: Yadav, A., Górszczyk, A., and Almeida, R.: Enhanced Subsurface Imaging of Western Nankai Trough Using Full Waveform Inversion, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21263, https://doi.org/10.5194/egusphere-egu25-21263, 2025.

GI5 – Earth surface and subsurface methods of investigation

EGU25-870 | Posters on site | GI5.1

Standard Penetration Test and Dynamic Cone Penetration Test Relationship for Coarse-Grained Soils 

Burak Tural, Tahir Yıldız, Yusuf Batuge, and Jad Alkhalifa

The Standard Penetration Test (SPT) is a commonly used and effective disturbed sampling in-situ method to obtain the strength characteristics of soils, providing significant results for geotechnical design. Several correlations between SPT blow counts (N value) and soil behavior have been established to define physical and mechanical properties, supporting the determination of design parameters for soil layers. Similarly, the Dynamic Cone Penetration Test (DCPT) is a feasible and cost-efficient method for assessing soil characteristics, providing continuous and time-conscious data. Obtaining correlations between SPT and DCPT can enhance data acquisition by leveraging the strengths of both methods. This study investigates the relationship between SPT and DCPT results for coarse-grained soils through a comprehensive site investigation conducted various locations in the Kingdom of Saudi Arabia (KSA) for a renewable energy project. The test points were almost identical, and a density-based relationship between SPT blow counts and DCPT penetration resistance was developed. Individual evaluation of relationship between SPT and DCPT conducted in site-specific conditions and the correlation of all sites combined and generalized together. The comparison of the proposed correlation and existing studies were utilized on similar conditions to validate reliability. An evaluation was made to correlate SPT-N&DCP (Blow/100mm) values with the results obtained from SPT&DCPT tests performed at four project sites. The correlation varies between 0.56 and 0.70. Combination of all sites calculated as 0.72. This research presents precious perceptions into incorporating SPT and DCPT data to optimize geotechnical design practices.

How to cite: Tural, B., Yıldız, T., Batuge, Y., and Alkhalifa, J.: Standard Penetration Test and Dynamic Cone Penetration Test Relationship for Coarse-Grained Soils, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-870, https://doi.org/10.5194/egusphere-egu25-870, 2025.

EGU25-2328 | Orals | GI5.1

An extension of the diffraction hyperbola method to layered media 

Raffaele Persico, Ding Yang, Gianfranco Morelli, Ilaria Catapano, Giuseppe Esposito, Gregory De Martino, and Luigi Capozzoli

The stratigraphy of urban sub-soils is commonly quite complex and the effective use of GPR technology requires a modelling of the signal propagation as occurring into a layered structure, often made up by not flat interfaces, rather than into a homogeneous medium. Accordingly, the estimate of the signal velocity into different materials needs to be accurate, because it affects both the focusing and the positioning of the buried targets [1-2]. In this framework, we propose an extension of the diffraction hyperbola method as effective tool for retrieving the propagation velocity of the electromagnetic waves in layered media [3]. In particular, we will consider a stratified soil with two layers whose separating interface is not flat. In this case, the diffraction curves are deformed by the refraction of the waves at the buried interface and no analytic formula for the scattering is available. We demonstrate that a suitable numerical forward modelling performed with the help of the gprMax software [4] can help retrieving the value of the propagation velocity in the second layer. At the conference we will show that, if properly dealt with, the diffraction curves generated by electrically small targets can still provide information about the properties of the soil, even if the reflection at the interface makes more difficult and trickier to look into the second layer. The method can be theoretically extended to a generic number of layers, but the possibility to effectively investigate targets in the third layer (or in layers following the third one) becomes practically feasible only if the reflection at the interfaces is weak, i.e. only if the electromagnetic characteristics of the subsequent adjacent layers are quite similar to each other.

Key words: Layered media, propagation velocity

References

[1] R. Pierri, G. Leone, F. Soldovieri, R. Persico, "Electromagnetic inversion for subsurface applications under the distorted Born approximation" Nuovo Cimento, vol. 24C, N. 2, pp 245-261, March-April 2001.

[2] I. Catapano, L. Crocco, R. Persico, M. Pieraccini, F. Soldovieri, “Linear and Nonlinear Microwave Tomography Approaches for Subsurface Prospecting: Validation on Real Data”, IEEE Trans. on Antennas and Wireless Propagation Letters, vol. 5, pp. 49-53, 2006.

[3] R. Persico G. Leucci, L. Matera, L. De Giorgi, F. Soldovieri, A. Cataldo, G. Cannazza, E. De Benedetto, Effect of the height of the observation line on the diffraction curve in GPR prospecting, Near Surface Geophysics, Vol. 13, n. 3, pp. 243-252, 2014.

[4] C. Warren, A. Giannopoulos, I Giannakis, gprMax: Open source software to simulate electromagnetic wave propagation for Ground Penetrating Radar, Computer Physics Communications, 209, 163-170, 2016 10.1016/j.cpc.2016.08.020.

How to cite: Persico, R., Yang, D., Morelli, G., Catapano, I., Esposito, G., De Martino, G., and Capozzoli, L.: An extension of the diffraction hyperbola method to layered media, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2328, https://doi.org/10.5194/egusphere-egu25-2328, 2025.

EGU25-2857 | Posters on site | GI5.1

GPR investigations at San Francesco di Paola ai Monti, Rome 

Raffaele Persico and Paolo Zimmaro

The St. Francis of Paola ai Monti church in Rome is an important historical building, currently (as of December 2024) closed to the public because of ongoing damage patterns causing structural damage (mainly cracks and fissures [1]). In view of the 2025 Jubilee, the Department of Environmental Engineering (DIAm) of the University of Calabria (Italy) was put in charge of geotechnical and geophysical analyses in order to assess the status of the building, understand the main causes of the ongoing structural problems, and address scientifically-informed restoration and retrofitting actions. In particular, we performed a Ground Penetrating Radar (GPR) investigation of the main nave and of three chapel on the right hand side looking toward the altar (this side is the most affected by fractures in the masonry). The investigation, as it often happens [2-4], has revealed several structural anomalies of cultural interest ascribable probably to tombs and mass graves. Some of these anomalies were deducible from inscriptions on the floor, while some others were not revealed by external traces. The data have been elaborated according to a well assessed linear data processing [5-6] and have also revealed the different consistency of the subsoil under one of the lateral chapels, which is coherent with the structural problems.

Key words: Structural investigations, cultural heritage

References

[1] P. Zimmaro, E. Ausilio, Geotechnical and structural investigation and monitoring techniques to determine the origin of ongoing damage processes in historical buildings: The Saint Francis of Paola Church in Rome case history, Geotechnical Engineering for the Preservation of Monuments and Historic Sites III – Lancellotta, Viggiani, Flora, de Silva & Mele (Eds), CRC Press, Napoli (Italy), June 22-24, 2022. DOI: 10.1201/9781003308867-47.

[2] R. Persico, S. D’Amico, L. Matera, E. Colica, C. de Giorgio, A. Alescio, GPR prospecting within the chapel of Aragon within the co-cathedral of St. John in Valletta, Malta, Proc. of 17th International conference on Ground Penetrating Radar, Rapperwil, Switzerland, June, 18-21, 2018.

[3] A. Calia, G. Leucci, M. T. Lettieri, L. Matera, R. Persico, M. Sileo, The mosaic of the crypt of St. Nicholas in Bari (Italy): Integrated GPR and laboratory diagnostic study, Journal of Archaeological Science, vol. 40, n. 12, pp. 4162-4169, December 2013.

[4] M. Pieraccini, L. Noferini, D. Mecatti, C. Atzeni, R. Persico, F. Soldovieri, Advanced Processing Techniques for Step-frequency Continuous-Wave Penetrating Radar: the Case Study of “Palazzo Vecchio” Walls (Firenze, Italy), Research on Nondestructive Evaluation, vol. 17, pp. 71-83, 2006.

[5] R. Pierri, G. Leone, F. Soldovieri, R. Persico, "Electromagnetic inversion for subsurface applications under the distorted Born approximation" Nuovo Cimento, vol. 24C, N. 2, pp 245-261, March-April 2001.

[6] I. Catapano, L. Crocco, R. Persico, M. Pieraccini, F. Soldovieri, “Linear and Nonlinear Microwave Tomography Approaches for Subsurface Prospecting: Validation on Real Data”, IEEE Trans. on Antennas and Wireless Propagation Letters, vol. 5, pp. 49-53, 2006.

How to cite: Persico, R. and Zimmaro, P.: GPR investigations at San Francesco di Paola ai Monti, Rome, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2857, https://doi.org/10.5194/egusphere-egu25-2857, 2025.

EGU25-4687 | Orals | GI5.1

Advanced airborne remote sensing methods for monitoring municipal solid waste landfills 

Olga Brovkina, František Zemek, Miroslav Pikl, Lukáš Fajmon, and Tomáš Fabiánek

Municipal solid waste (MSW) landfills are dynamic environments where biological, chemical, and physical processes such as waste decomposition, gas emissions, and settlement create complex challenges for monitoring and management. Effective landfill management requires comprehensive and reliable information on key factors such as landfill volume, the distribution and health of herbaceous vegetation, including invasive species, and the spatial dynamic of active waste deposition zones. Advanced remote sensing technologies, particularly airborne hyperspectral (HS) imaging in the visible, near-infrared, shortwave infrared (VNIR, SWIR), and thermal infrared (TIR) regions, and airborne laser scanning (ALS) offer a powerful approach to addressing these challenges.

This study demonstrates the potential of the airborne hyperspectral VNIR-SWIR and TIR data and ALS-derived DEMs (https://olc.czechglobe.cz/en/flis-2/) for monitoring two active MSW landfills in the Czech Republic. A key focus of this research is the integration of airborne data processing with ground-based surveys to improve the accuracy of landfill volume assessments and vegetation monitoring. The ground-based survey included precise GPS measurements and detailed botanical survey on landfills. High spectral resolution data from VNIR and SWIR sensors enable detailed characterization of landfill vegetation, including the identification of herbaceous species and the detection of invasive plants based on their spectral signatures. Additionally, TIR imaging provides information about surface temperature anomalies, which can indicate active waste zones and areas of increased methane emissions.

ALS data, used for generating high-resolution DEMs, allow for precise delineation of landfill boundaries, accurate estimation of landfill volume, and detection of settlement or landslide patterns. When integrated with hyperspectral data, the DEMs help refine vegetation filtering algorithms, improving elevation accuracy in areas with dense herbaceous cover.

The proposed methodology of landfill monitoring provides detailed spatial and temporal insights that are critical for decision-making. These findings underscore the transformative potential of hyperspectral, thermal infrared, and airborne laser scanning technologies in supporting the effective and sustainable management of MSW landfills, providing a valuable tool for ecological monitoring, environmental risk assessment, and operational optimization.

Key words: hyperspectral, thermal, laser scanning, herbaceous vegetation, volume, sustainable management

Acknowledgement: The research is supported by the Technology Agency of the Czech Republic grant number SS06020164, and the Ministry of Education, Youth and Sports of the Czech Republic within the CzeCOS program, grant number LM2023048.

How to cite: Brovkina, O., Zemek, F., Pikl, M., Fajmon, L., and Fabiánek, T.: Advanced airborne remote sensing methods for monitoring municipal solid waste landfills, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4687, https://doi.org/10.5194/egusphere-egu25-4687, 2025.

EGU25-5509 | Posters on site | GI5.1

EMILI project: ElectroMagnetic techniques for Investigating Landslide and structural damages due to their Impacts on the bridges 

Luigi Capozzoli, Gregory De Martino, Giuseppe Salvia, Davide Di Gennaro, Valeria Giampaolo, Angela Perrone, Ilaria Catapano, Giovanni Ludeno, Giuseppe Esposito, Gianluca Gennarelli, Alessandro Giocoli, Chiara Ormando, Antonio Di Pietro, Maurizio Pollino, Giacomo Buffarini, and Paolo Clemente

Bridges and viaducts are critical elements of transportation infrastructure, and ensuring their structural integrity is vital for safety and functionality. These structures are susceptible to damage from natural events, like landslides, or from human-made accidents, which can lead to severe consequences such as structural collapses, traffic disruptions, and safety risks. The severity of these impacts depends on factors such as the type of landslide and the design and condition of the infrastructure. Evaluating landslide risks requires a thorough assessment of various factors, including the geophysical properties of the soil and the condition of key structural elements of the bridge or viaduct, such as foundations, piers, and abutments. Remote and in-situ electromagnetic technologies are increasingly employed for this purpose, but there is currently no standardized protocol for their effective application. Existing risk assessments are often inconsistent, varying from case to case and heavily relying on the expertise of the operators. Moreover, the effectiveness of each electromagnetic technology is influenced by the specific scenario, the devices used, and the user's skill in interpreting the data. The EMILI project aims to address these challenges by developing standardized guidelines, best practices, and protocols for the use of electromagnetic technologies in assessing landslide risks for bridges and viaducts. The project has two primary goals: (1) to conduct a systematic review of the performance of available remote and in-situ electromagnetic technologies, and (2) to advance the use of electrical and electro-magnetic geophysical methodologies for investigating bridge foundations and structural assessments. The EMILI project is funded by the FABRE consortium, a technical and scientific Italian alliance for monitoring, promoting and assessing the safety of bridges and viaducts in Italy

How to cite: Capozzoli, L., De Martino, G., Salvia, G., Di Gennaro, D., Giampaolo, V., Perrone, A., Catapano, I., Ludeno, G., Esposito, G., Gennarelli, G., Giocoli, A., Ormando, C., Di Pietro, A., Pollino, M., Buffarini, G., and Clemente, P.: EMILI project: ElectroMagnetic techniques for Investigating Landslide and structural damages due to their Impacts on the bridges, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5509, https://doi.org/10.5194/egusphere-egu25-5509, 2025.

EGU25-6821 | Posters on site | GI5.1

Time and space variability of spectral ratio in urban area: the case of Rome (Italy) 

Alessia Mercuri, Giovanna Cultrera, Maurizio Vassallo, Giuseppe Di Giulio, Antonella Bobbio, and Gaetano Riccio

Studies in urban areas are becoming increasingly important for the ground motion prediction, and represent a stimulating challenge due to the presence of many uncontrolled variables: high and variable level of ambient noise, hidden geological features, underground services, limited open spaces for geophysical investigations, high urbanisation and cultural heritage. 

We used data from 24 stations in the urban area of Rome (Italy), belonging to the SPQR temporary seismic network and operating from January to early April 2021 (https://www.fdsn.org/networks/detail/7M_2021/). The stations were installed on very different geological conditions with the aim to reconstruct the properties of the propagation medium below the city by interferometric analysis based on cross correlation of ambient noise. 

The recorded continuous data allowed us to study the network performance in terms of detection threshold for earthquakes and the noise variability over the time during the pandemic restriction due to Covid-19. In particular, we investigated the spatial and temporal variation of the Horizontal to Vertical Spectral ratio on noise (HVSR) computed with the HVNEA software (https://github.com/INGV/hvnea). The coherence analysis between the time series of the HVSR frequency peak values and their related amplitude shows an anti-correlation between the two parameters. Their variability is compared with the total number of vehicles, detected by control units in the all metropolitan area and affected by the movement restrictions imposed by the public authority to contain Covid 19 infections: the correlation is significant in the medium-high frequency range but with different characteristics from site to site; no variations linked to traffic are observed in the low frequency range. 

Following these results, a permanent network of 14 stations, equipped with both velocimeter and accelerometer, is being installed in Rome by the Site Effect Laboratory of INGV (https://www.ingv.it/en/monitoraggio-e-infrastrutture/laboratori/laboratorio-effetti-di-sito), as part of the MEET Project (Monitoring Earth's Evolution and Tectonics, https://meet.ingv.it; National Recovery and Resilience Plan- PNRR). The network will be devoted to site effect studies in such an urban area with unique cultural heritage and heterogeneous city development.

How to cite: Mercuri, A., Cultrera, G., Vassallo, M., Di Giulio, G., Bobbio, A., and Riccio, G.: Time and space variability of spectral ratio in urban area: the case of Rome (Italy), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6821, https://doi.org/10.5194/egusphere-egu25-6821, 2025.

EGU25-8209 | ECS | Orals | GI5.1

Geophysical monitoring of river levees infrastructure 

Paola Boldrin and Enzo Rizzo

As extreme weather events like heavy rainfall, storms, and flooding become more frequent and intense due to climate change, levees are put under increasing pressure. River levees play a crucial role in safeguarding human lives and economic activities, acting as vital barriers against such extreme events. The main causes of embankment failure include both external and internal erosion, as well as instability, primarily driven by the strong water pressure exerted during river floods. Additionally, other meteorological phenomena, human activities, and the presence of animals or certain types of vegetation can weaken levees, contributing to instability, subsidence, or breakage. To mitigate these risks and ensure the long-term safety of levees, regular maintenance, preventative measures, and the implementation of advanced monitoring systems are essential to detect early signs of weakness and structural instability. Geophysical methods could play a vital role in assessing the integrity and stability of levees, providing essential data for their design, maintenance, and monitoring. Additionally, these methods are non-invasive, allowing for frequent and cost-effective monitoring without disrupting levee functionality. Ultimately, the integration of geophysical data with engineering assessments enhances levee safety, ensuring better flood protection. In the past years, the geophysical prospection methods have been improved for the inspection of levees infrastructure in order to detect the heterogeneity, which should be the critical aspects destabilizing the hydraulic system. Anyway, the potential of geophysical techniques in levees is mainly known in characterisation contexts, while a monitoring use has not yet been developed. Therefore, new applications and laboratory experiments are needed to enhance their capability and development. Therefore, new applications and laboratory experiments are needed to enhance their capabilities and development. Additionally, leveraging advancements in real-time data acquisition and interpretation technologies could improve the overall accuracy of the monitoring system, enabling earlier detection of potential issues and more effective management of preventive measures. This work introduces several geophysical applications on different levees taking in account internal heterogeneities, hydraulic infiltration, natural cavities and levees stability. Different geophysical methods were used: Electromagnetic methods (FDEM and GPR), Electrical Resistivity Tomography and Self Potential monitoring. The application was performed to monitor the effectiveness of the consolidation beneath the building with time. In addition, an experiment was carried out in the laboratory through the creation of a physical model of a levees where different simulations were disposed in order to improve the geophysical analysis.

How to cite: Boldrin, P. and Rizzo, E.: Geophysical monitoring of river levees infrastructure, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8209, https://doi.org/10.5194/egusphere-egu25-8209, 2025.

EGU25-9202 | Orals | GI5.1 | Highlight

Rapid and non-invasive structural characterization of the Roman Arena in Verona, Italy, through geophysical prospecting 

Maria Rosaria Gallipoli, Nicola Tragni, Giovanni Gangone, Vincenzo Serlenga, and New Age working group

The current Italian guidelines dedicated to monumental assets do not delve into issues related to the characterization of the overall above-soil system and the enhancement of archaeological structures buried below the monumental asset. Furthermore, the guidelines for seismic microzonation focus only on seismotectonic, lithostratigraphic and geotechnical characterization of surface soils, completely neglecting the presence of the built environment. Ground motion and structural response of built environment are treated separately. This aspect can be significantly limiting in historic centres, where heritage buildings rest on numerous subsurface layers of buried structures in an extensively modified subsoil. In this context, the Italian NEW AGE project (PRIN 2022 “NEW integrated approach for seismic protection and valorisation of heritAGE buildings on historical soil deposits”) aims to fill some gaps; during this project, we adopted a multiscale and multi-resolution geophysical approach to investigate geological sub-surfaces, soil/foundations environments and cultural heritage structures and their interactions with each other as a single complex soil-building system by adopting a holistic view. We have tested this approach on two monumental assets of inestimable value, such as the Roman Arena of Verona (Northern Italy) and the Santa Sofia bell tower in Benevento (Southern Italy).

Here we report the first results of MASW, ESAC, of 60 single-station and 9 array seismic prospecting conducted on both the soil and in the Arena. The investigations conducted on the foundation soil and on surrounding the Arena allowed for the mechanical and seismo-stratigraphic characterization of the subsoil, while the surveys carried out within the Arena enabled the estimation of the main structural parameters (vibrational modes, modal shapes, and seismic noise wave propagation velocities) at multiple points of the structure. The main advantages of these surveys are the ease of execution and total non-invasiveness, which makes it possible to characterize even large monumental properties and to carry out the surveys at any time of the day, even during tourist visits.

How to cite: Gallipoli, M. R., Tragni, N., Gangone, G., Serlenga, V., and working group, N. A.: Rapid and non-invasive structural characterization of the Roman Arena in Verona, Italy, through geophysical prospecting, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9202, https://doi.org/10.5194/egusphere-egu25-9202, 2025.

EGU25-9888 | Posters on site | GI5.1

Advanced GPR Imaging in layered media  

Gregory De Martino, Ding Yang, Gianfranco Morelli, Ilaria Catapano, Giuseppe Esposito, Luigi Capozzoli, and Raffaele Persico

The effective use of Ground Penetrating Radar (GPR) in urban environment benefits of the ability to manage data referred to a layered scenario. The GPR imaging in layered media can be improved either making use of focusing algorithms [1-2] accounting in a rigorous way for the layered structure of the soil or, more simply and less demandingly from the point of view of the available computing resources, making use of a joined migration and of a combined time-depth conversion of the data [3-4]. These recently introduced possibilities allow to deal with layered media as homogeneous ones. The inhomogeneity of the investigated medium is, indeed, accounted for through a sort of sticking of different results and with some suitable deformation of the resulting image. Advantages of the combined time-depth conversion but also its intrinsic limits will be discussed. For example, it is helpful for the correct imaging of cavities [5] allowing, in a simple and straightforward way, the mitigation of the well-known compression effect that the cavities suffer in a classical GPR imaging. This claim is supported by both numerical results obtained from data simulated with the gprMax software [6] and by experimental results obtained in real test scenarios.

Key words: Layered media, joined migration, combined time-depth conversion

References

[1] R. Pierri, G. Leone, F. Soldovieri, R. Persico, "Electromagnetic inversion for subsurface applications under the distorted Born approximation" Nuovo Cimento, vol. 24C, N. 2, pp 245-261, March-April 2001.

 

[2] I. Catapano, L. Crocco, R. Persico, M. Pieraccini, F. Soldovieri, “Linear and Nonlinear Microwave Tomography Approaches for Subsurface Prospecting: Validation on Real Data”, IEEE Trans. on Antennas and Wireless Propagation Letters, vol. 5, pp. 49-53, 2006.

 

[3] R. Persico, G. Morelli, G. Esposito, I. Catapano, L. Capozzoli, G. De Martino, D. Yang, An innovative time-depth conversion for the management of buried scenarios with strong discontinuities, Journal of Applied Geophysics vol. 227, 105435, DOI 10.1016/j.jappgeo.2024.105435, 2024.

 

[4] D. Yang, L. Capozzoli, I. Catapano, G. De Martino, G. Esposito, G. Morelli and R. Persico, Accounting for the Different Propagation Velocities for the Focusing and Time–Depth Conversion in a Layered Medium, Applied Sciences 14(24):11812, 2024.

 

[5] R. Persico, S. D'Amico, L. Matera, E. Colica, C. De, Giorgio, A. Alescio, C. Sammut and P. Galea, GPR Investigations at St John's Co‐Cathedral in Valletta. Near Surface Geophysics, vol. 17 n. 3, pp. 213-229. doi:10.1002/nsg.12046, 2019.

 

[6] C. Warren, A. Giannopoulos, I Giannakis, gprMax: Open source software to simulate electromagnetic wave propagation for Ground Penetrating Radar, Computer Physics Communications, 209, 163-170, 2016 10.1016/j.cpc.2016.08.020.

 

How to cite: De Martino, G., Yang, D., Morelli, G., Catapano, I., Esposito, G., Capozzoli, L., and Persico, R.: Advanced GPR Imaging in layered media , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9888, https://doi.org/10.5194/egusphere-egu25-9888, 2025.

Urban seismology has emerged as a distinct field for understanding the close interactions between human activities and the near-surface environment, particularly in densely populated regions. This presentation shares research experiences and insights from Singapore, a highly urbanized and dynamic setting. We examine case studies demonstrating the versatility of urban seismic methods in addressing engineering, environmental, and geophysical questions. These include using ambient noise monitoring for mapping bedrock interfaces, mitigating construction risks during tunneling, characterizing reclaimed land, and quantifying urban activities. By leveraging a combination of nodal seismometers and distributed acoustic sensing (DAS), our work has provided high-resolution subsurface models and continuous monitoring capabilities tailored to urban needs.

However, unique challenges arise in urban environments, including complex and temporally varying noise sources, limited sensor deployment options, and non-linear interactions between seismic waves and infrastructure. These issues are further compounded by the need to adapt conventional active and interferometric seismic workflows to account for heterogeneous urban conditions and to achieve meaningful resolutions for shallow subsurface features.

Our findings from Singapore underscore the potential of urban seismology to inform city planning, hazard mitigation, and sustainable infrastructure development. At the same time, they emphasize the necessity of developing innovative techniques and data processing strategies to overcome the complexities of urban noise and constrained observational settings. These learnings provide a foundation for extending urban seismology applications to other metropolitan regions worldwide.

How to cite: Li, Y. E.: Applications and challenges of urban seismology - learnings from Singapore, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9970, https://doi.org/10.5194/egusphere-egu25-9970, 2025.

EGU25-10055 | Orals | GI5.1

Combined GPR and ERT prospecting for non-invasive investigation of the Roman Amphitheater in Verona (Italy) and its surroundings  

Capozzoli Luigi, Gregory De Martino, Giuseppe Calamita, Jessica Bellanova, Sabatino Piscitelli, Angela Perrone, Luigi Martino, and Maria Rosaria Gallipoli

The Italian NEW AGE project (PRIN 2022 “New Integrated Approach for Seismic Protection and Enhancement of Heritage Buildings on Historic Earthen Deposits”) seeks to advance seismic risk mitigation strategies for all cities with significant monumental heritage and all historic centres.

The project adopts a holistic approach, treating the urban environment as an integrated soil-building system, to assess and address the mutual interactions between subsurface conditions and overlying cultural heritage structures. This approach is crucial for the effective preservation of heritage sites in seismic-prone areas.

Seismic investigations, integrated with electromagnetic (GPR) and electrical resistivity tomographies (ERTs), provide non-invasive methods suitable for investigating subsurface conditions and foundation structures beneath urban environments. GPR is particularly effective for characterizing  the shallower layers of subsoil and for detecting possible buried archaeological features. Similarly, ERT is a robust and cost-effective method for delineating the geometry of geological structures in urban areas, at greater depths.

The project employs a multiscale, multiresolution geophysical strategy to comprehensively study the geological subsurface, soil-foundation systems, and heritage structures. By integrating these methods, the PRIN NEW AGE project aims to provide a robust framework for seismic risk mitigation and the sustainable preservation of cultural heritage in urban areas. The proposed strategy was tested to characterize the subsurface of the Arena di Verona from an archaeological and geological point of view, through the combined and integrated use of Seismic, GPR and ERT. In this presentation, only the results obtained with GPR and ERT will be presented while the seismic analyses will be presented by Gallipoli et al. in the work “Rapid and non-invasive structural characterization of the Roman Arena in Verona, Italy, through geophysical prospecting”. 

GPR acquisitions were performed with a monochannel system coupled to antennae operating at different frequencies, and a multichannel GPR stepped-frequency system equipped with an external GNSS system.  GPR data collected by the first GPR system, operating at frequencies of 200 and 400 MHz, allowed the identification of the Arena foundation system, while the multichannel system, leveraging the unmatched resolution offered, enabled the identification of interesting anomalies within the amphitheatre and surrounding areas, belonging to different historical phases.

ERTs  were carried inside the Arena and in Piazza Bra. In Piazza Bra, two ERTs were conducted with a 5-meter electrode spacing, covering a total length of 235 meters, to investigate depths of up to several tens of meters for geological purposes while, in the Cavea, two ERTs  were conducted in two different arcades, along with a roll-along ERT survey in the longitudinal tunnel beneath the Cavea for improving the resolution and supporting the archaeological research.

The information obtained with GPR and ERTs, supported and validated by archaeological data and geotechnical drilling have provided highly valuable insights from both the engineering and the archaeological perspectives.

Geophysical activities are realized also exploiting instrumentations and facilities provided by the Research Infrastructures of IRPAC (financed by PO FESR Basilicata 2014-2020 – DGR n. 402 del 28.06.2019 / CUP: G29J19001190003) and ITINERIS (financed by European Union – Next Generation EU, PNRR, M4C2 inv.3.1, CUP B53C2200215000).

 

How to cite: Luigi, C., De Martino, G., Calamita, G., Bellanova, J., Piscitelli, S., Perrone, A., Martino, L., and Gallipoli, M. R.: Combined GPR and ERT prospecting for non-invasive investigation of the Roman Amphitheater in Verona (Italy) and its surroundings , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10055, https://doi.org/10.5194/egusphere-egu25-10055, 2025.

EGU25-12912 | Posters on site | GI5.1

Advances in Seismic Risk Assessment of the city of Potenza (Southern Italy) 

Giovanni Gangone, Maria Rosaria Gallipoli, and Marco Vona

The overall objective of this study is to improve the seismic risk assessment of the city of Potenza (southern Italy, selected because it is already the subject of several national and international research projects) based on a multidisciplinary approach that considers the seismic hazard of soils in the urban area, the interaction effect between soils and buildings, and the seismic capacity of buildings. 453 (300 on soils and 153 on buildings) single-station ambient noise measurements analysed through Horizontal-to-Vertical Spectral Ratio technique have been performed to assess the main characteristics of the most representative litho-stratigraphic and mechanical conditions of the urban soil and built environment in the city of Potenza. The main peak of the first vibrational frequency of the urban soils (f0s) mainly varies between 1.1 and 9.5 Hz, with a median value of 3.5 Hz; interpolating these measured points by the Kriging method, the map of the main frequency at each urban soil point was obtained. The first vibrational frequency of the 153 measured buildings (f0b) varies between 1.2 and 6.5 Hz; the experimental relationship between period, height and building area, derived by experimental results, made it possible estimating the fundamental frequency for all the Potenza's buildings. By comparing the frequency ranges of buildings with those of foundation soils, it was possible to spatially determine the areas and probabilities of highest occurrence of the soil-building resonance effect in the elastic field throughout the city of Potenza.

Furthermore, capacity curves of buildings were obtained based on the geometric and typological characteristics and on the vibrational frequencies of the measured building. Firstly, the buildings were grouped into homogeneous classes. Based on previous and well-established principles and studies, they were distinguished by construction year (pre-1971, post-1971), presence of soft stories, and number of stories. The capacity curves for each typology were defined in terms of the top displacement – base shear relationship.  The values for the yield displacement (δy) and the ultimate displacement (δu) were calculated based on the values obtained from numerical modelling of previous studies. For each of the considered typology, a mean capacity curve was obtained by averaging the values of the buildings belonging to each class. This approach provides a first seismic assessment of the seismic response of buildings, starting from the measured frequencies and considering the influence of different geometric and typological characteristics. The capacity curves obtained can be used as valuable tools to assess the vulnerability of these buildings and define a seismic risk map for the city of Potenza including the urban soil amplification and the soil-building interaction effect. 

How to cite: Gangone, G., Gallipoli, M. R., and Vona, M.: Advances in Seismic Risk Assessment of the city of Potenza (Southern Italy), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12912, https://doi.org/10.5194/egusphere-egu25-12912, 2025.

EGU25-12920 | Posters on site | GI5.1

Integrated geophysical methodology for subsurface modeling and seismic response analysis in the Campi Flegrei area 

Silvia Giallini, Maurizio Simionato, Federica Davani, Iolanda Gaudiosi, Marco Mancini, Amerigo Mendicelli, Massimiliano Moscatelli, Federica Polpetta, Daniel Tentori, and Francesco Stigliano

The Campi Flegrei area, located in southern Italy, is characterized by complex geological stratigraphy and elevate seismic and volcanic risks, exacerbated by ongoing bradyseismic phenomena.

This region, located in a densely populated context, poses significant challenges for seismic hazard assessment due to its geological complexity, frequent seismic activity and the vulnerability of infrastructures

The recently recorded seismic swarms, including those of 2023, further highlight the need for accurate subsurface characterization to assess and mitigate seismic risks.

In this context, a geophysical campaign is being conducted as part of a larger project aimed at advancing seismic microzonation and providing detailed data for risk mitigation strategies. This contribution focuses on the application of an integrated geophysical methodology for reconstructing a detailed subsurface model for local seismic response analysis at several sites of particular interest for civil protection purposes in the Campi Flegrei area.

In this study, new geophysical data were acquired and then processed through integration with geological data. Geophysical surveys include both passive seismic measurements, carried out with single-station and array configurations, and active seismic testing using the Multichannel Analysis of Surface Waves (MASW) method. These passive and active seismic techniques yield information on shear-waves velocity profiles and subsurface heterogeneities.The ongoing analyses aim to explore the characteristics of the volcanic subsurface, contributing to a better understanding of its structural complexity. A strong emphasis is placed on integrating geophysical and geological data to improve the resolution and accuracy of the subsurface model.

This work highlights the critical role of non-invasive geophysical methodologies, such as passive and active seismic methods, in urban and volcanic areas. These efforts support the strategic objectives of urban geophysics by promoting urban resilience and sustainability, while also providing actionable insights for prevention and urban planning in the Campi Flegrei area.

By integrating advanced geophysical techniques, this research enhances the understanding of subsurface properties and their interaction with seismic phenomena, laying the foundation for effective risk mitigation and resilience-building measures in this highly complex and dynamic region.

How to cite: Giallini, S., Simionato, M., Davani, F., Gaudiosi, I., Mancini, M., Mendicelli, A., Moscatelli, M., Polpetta, F., Tentori, D., and Stigliano, F.: Integrated geophysical methodology for subsurface modeling and seismic response analysis in the Campi Flegrei area, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12920, https://doi.org/10.5194/egusphere-egu25-12920, 2025.

EGU25-16519 | Orals | GI5.1

Integrated geophysical approaches for geo-hazards evaluation in urban areas: activities in urban sites of Basilicata and Campania region (southern Italy) 

Valeria Giampaolo, Vincenzo Serlenga, Gregory De Martino, Giovanni Gangone, Luigi Martino, Giuseppe Calamita, Maria Rosaria Gallipoli, Iolanda Gaudiosi, Angela Perrone, Tony Alfredo Stabile, and Vincenzo Lapenna

The WP7 - GEOSPHERE-LANDSURFACE of the ITINERIS project (Italian Integrated Environmental Research Infrastructures System, PNRR M4C2 Inv.3.1 IR), funded by the European Union – Next Generation EU, aims to provide openly accessible digital data on the solid Earth to the scientific community, the public, and decision-makers in line with the Digital Earth concept.

Specifically, Activity 7.4 is dedicated to developing an integrated multi-scale, multi-resolution, and multi-sensor approach for characterizing the surface, subsurface, and built environment in urban areas, as well as monitoring civil infrastructure of strategic importance to mitigate the impacts of natural and anthropogenic hazards.

After an initial phase of geophysical equipment upgrades, the advanced instruments have been tested at the project’s pilot sites: the urban area of Potenza, which faces high seismic risk, and the peri-urban area in the municipality of Tito (PZ), affected by a slow-moving landslide. Furthermore, ITINERIS geophysical equipment is contributing to the scientific activities of the project NEW AGE (funded by the European Union – Next Generation EU), aimed at the seismic protection and valorisation of cultural heritage buildings in the historical centre of Benevento (Campania, Italy). Joint seismic noise and deep electrical resistivity studies are also underway in the municipality of Contursi Terme (SA) as part of the project TOGETHER, also funded by the European Union – Next Generation EU, focused on the sustainable exploitation of geothermal resources. Finally, ITINERIS geophysical equipment will be utilized in the Seismic Microzonation studies of the Campi Flegrei area for the Italian Civil Protection Department.

The study areas, characterized by high levels of seismic and hydrogeological risk, will benefit from the joint geophysical analyses conducted using the innovative equipment provided by the infrastructure. It is expected that the multi-geophysical approach developed within the framework of the ITINERIS project will contribute to the definition of a more accurate subsurface model, which, in turn, will be highly advantageous for the assessment of the actual hazards in the study areas. Furthermore, in certain specific locations, the approach may also support a more reliable evaluation of geothermal resources.

How to cite: Giampaolo, V., Serlenga, V., De Martino, G., Gangone, G., Martino, L., Calamita, G., Gallipoli, M. R., Gaudiosi, I., Perrone, A., Stabile, T. A., and Lapenna, V.: Integrated geophysical approaches for geo-hazards evaluation in urban areas: activities in urban sites of Basilicata and Campania region (southern Italy), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16519, https://doi.org/10.5194/egusphere-egu25-16519, 2025.

EGU25-18868 | Posters on site | GI5.1

Geophysical investigations supporting a 3D model reconstruction in the historical center of Rome: WP2-PREDICT Project  

Daniela Famiani, Paola Bordoni, Fabrizio Cara, Michele Cercato, Giuseppe Di Giulio, Fabrizio Marra, Giuliano Milana, Stefania Pucillo, Gaetano Riccio, Maurizio Vassallo, Gianluca Chessa, Giovanna Cultrera, Salomon Hailemikael, Alessia Mercuri, Teresa Tufaro, Federica Di Michele, and Daniele Silvestri

The historical center of Rome, due to the presence of a priceless cultural heritage, needs to be protected by natural risks including the seismic one. It is hence important to study the seismic response of downtown Rome in detail to estimate shaking levels in case of an earthquake. 

As widely known, to investigate the subsoil characteristics of a very highly urbanized area, geophysical techniques are the most effective, especially in the presence of ancient buildings which cannot be damaged by using invasive techniques. The new portable nodal seismic sensors, recently acquired by INGV, feature a compact, self-contained, autonomous land wireless seismic data acquisition system, making them well suited for use in urban environments.

In the framework of the PREDICT project (Progetto INGV Pianeta Dinamico St-Predict), WP2 aims to constrain the complex shallow geophysical subsoil model of a part of the urban centre of Rome as input for a reliable 3D model of the area to finalise the study of the seismic response in a range of frequencies of engineering interest.

Many geophysical campaigns were performed using the nodal sensors in sites selected based on the geological reconstruction of the area, in order to estimate the seismic characteristics of the subsoil for the different sites. Ambient noise measurements in a single station or array configuration were performed, together with downhole investigations.

In this work we show the results obtained in terms of microtremor spectral ratios curves (HVNSR) and velocity profiles correlated with the geological succession in order to identify possible lateral lithological variabilities which can significantly affect the expected seismic response.

How to cite: Famiani, D., Bordoni, P., Cara, F., Cercato, M., Di Giulio, G., Marra, F., Milana, G., Pucillo, S., Riccio, G., Vassallo, M., Chessa, G., Cultrera, G., Hailemikael, S., Mercuri, A., Tufaro, T., Di Michele, F., and Silvestri, D.: Geophysical investigations supporting a 3D model reconstruction in the historical center of Rome: WP2-PREDICT Project , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18868, https://doi.org/10.5194/egusphere-egu25-18868, 2025.

EGU25-20094 | Orals | GI5.1

Gravity and GPR modeling of the subsurface structures below the Basilica dello Spirito Santo in Naples (Italy)  

Maurizio Fedi, Maurizio Milano, Mauro La Manna, Luigi Bianco, and Valentina Russo

This study aims at the interpretation and modeling of the subsurface anthropic structures below the Basilica dello Spirito Santo  in Naples (Italy) through the acquisition and processing of microgravimetric and GPR data. The analysis of GPR data provides significant information about buried elements and architectural stratifications, compatible with interventions from the past. In particular, several cavities were identified and interpreted as graves. However, this method did not image clearly the presence of the church foundation. In addition, we computed the vertical gradient of the gravity data in order to enhance the contributions due to subsurface structures. We then performed a multiscale imaging (multiridge method)  to estimate the depth and geometry of the sources. This analysis revealed that at a depth of about 0.5-1 m, there are several cavities, tombs, shafts, in agreement with GPR data. Most importantly, we also detected at about 5 m depth a rectangular structure that can be interpreted as the church foundation.

Our results demonstrate that the combination of GPR and gravity surveys is a successful strategy to detect subsurface anthropogenic structures in urban areas. In particular, the gravity method proved to be more effective to infer information about the deep church foundations which were questioned, while simultaneously detecting the subsurface cavities that can be attributed to tombs.

How to cite: Fedi, M., Milano, M., La Manna, M., Bianco, L., and Russo, V.: Gravity and GPR modeling of the subsurface structures below the Basilica dello Spirito Santo in Naples (Italy) , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20094, https://doi.org/10.5194/egusphere-egu25-20094, 2025.

EGU25-20313 | ECS | Orals | GI5.1

High-resolution time-lapse DC-IP imaging of a green infrastructure’s response to a flooding test and a heavy rain event 

Alexis Luzy, Adrien Dimech, François Duhaime, Jean-Sébastien Dubé, Janie Masse-Dufresne, and Rose-Anne Farley

Stormwater management is an escalating challenge in urban areas worldwide. Green Infrastructures (GIs), such as vegetated roadside areas with lowered curbs, are gaining recognition in Quebec as an effective solution to reduce the burden on urban sewage systems. However, the widespread use of de-icing salt during winter raises concerns about increased contaminant infiltration into the ground, potentially leading to infrastructure deterioration. Despite the growing adoption of GIs, a research gap persists regarding their impact on water and chloride infiltration.
In this study, a 50m-long GI was equipped with a large range of hydrogeological sensors such as water content and pore pressure sensors, thermistors, barometer and piezometers equipped with level, temperature and conductivity loggers. In addition, a time-lapse electrical resistivity tomography (TL-ERT) monitoring system was installed to extend spatially and temporally the coverage of the hydrogeological monitoring of the GI. In total, 113 electrodes were installed in boreholes and connected to an autonomous resistivity meter. In this study, 64 electrodes located within and around a 6m × 1.8m grid were used to recover the spatial and temporal distribution of electrical resistivity perpendicularly to the GI.
A controlled flooding test (CFT) using bromide salt as a saline tracer was conducted to evaluate the GI’s response to infiltration. A multi-method surveying and sampling program was implemented, integrating ERT and induced polarization (IP) geophysical measurements, hydrogeological monitoring (piezometers), and geochemical analyses (continuous groundwater sampling). In addition, a heavy rainfall event (HRE) was monitored using DC-IP surveys conducted every two hours. In total, approximately 90 DC surveys were completed during the CFT, with a temporal resolution of approximately 10 minutes and 50 DC-IP surveys were performed during the HRE, with a temporal resolution varying  from 2 to 4 hours. 
This study presents geophysical imaging results from these events, showcasing time-lapse imaging interpreted using laboratory analyses of the soil in-situ. Preliminary results suggest that the geophysical results are consistent with hydrogeological and geochemical data, offering valuable insights into the 2D distribution and temporal evolution of water and chloride movement in and around the GI. These findings contribute to understanding the performance and potential limitations of GIs in mitigating stormwater impacts under saline conditions.

How to cite: Luzy, A., Dimech, A., Duhaime, F., Dubé, J.-S., Masse-Dufresne, J., and Farley, R.-A.: High-resolution time-lapse DC-IP imaging of a green infrastructure’s response to a flooding test and a heavy rain event, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20313, https://doi.org/10.5194/egusphere-egu25-20313, 2025.

EGU25-828 | ECS | Orals | GI5.2 | Highlight

Advancing Mine Safety through Integrated Geophysical Techniques: A Pathway to Sustainable and Risk-Free Mining Practices 

Rajwardhan Kumar, Amit Bera, Sanjit Kumar Pal, and Ram Madhav Bhattacharjee

Mining plays a critical role in economic development, yet it presents significant safety risks and environmental challenges. Balancing worker safety and environmental preservation while maintaining sustainable practices is a pressing concern for the modern mining industry. This study explores the use of integrated geophysical techniques to enhance mine safety assessments and support sustainable mining operations. By combining methods such as Electrical Resistivity Tomography (ERT), seismic surveys, Ground-Penetrating Radar (GPR), magnetic surveys, and gravity surveys, the approach provides a comprehensive and non-invasive understanding of subsurface conditions in active mining areas. The integrated geophysical framework enables real-time monitoring of underground stability, facilitating the detection of hazards such as ground subsidence, roof falls, sinkholes, potholes, and unstable fault zones. These techniques deliver high-resolution data, revealing surface and deep structural instabilities, which allow for proactive risk management and inform strategic decision-making processes. The research demonstrates how continuous geophysical monitoring reduces accident risks, enhances operational efficiency, and ensures long-term sustainability in mining practices. This study further highlights the broader benefits of adopting integrated geophysical methods, emphasizing their role in minimizing environmental impact while improving workplace safety. By integrating advanced geophysical techniques into mining operations, this research establishes a model for ensuring both worker safety and environmental preservation, aligning with global sustainable development goals. The proposed approach bridges the gap between mining safety and sustainability, showcasing the potential of technological innovation to mitigate the inherent risks of mining activities.

How to cite: Kumar, R., Bera, A., Pal, S. K., and Bhattacharjee, R. M.: Advancing Mine Safety through Integrated Geophysical Techniques: A Pathway to Sustainable and Risk-Free Mining Practices, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-828, https://doi.org/10.5194/egusphere-egu25-828, 2025.

EGU25-2727 | Orals | GI5.2

Automated BIM Reconstruction from Point Clouds Using IFC Standards in Indoor Environment 

Ruoming Zhai, Xiaoqing Gan, Yifeng He, and Jianzhou Li

Point cloud data acquired through LiDAR technology enables the rapid reconstruction of complex indoor building structures. However, due to the discrete nature of point clouds, they fail to accurately represent the geometric dimensions of building components and cannot be directly applied to digital model construction. Conventionally, this limitation necessitates manual modeling in specialized BIM software to integrate both geometric and semantic information of building structures, which is labor-intensive and time-consuming. To address this, we propose an automated method for geometric feature extraction and BIM reconstruction, enabling more efficient and accurate modeling processes. By segmenting building components and extracting their geometric features, the method automates the construction of building structural entities based on the IFC (Industry Foundation Class) standard, which is an open and vendor-neutral modeling standard widely used in the BIM domain.

Specifically, the approach starts by filtering ceilings and floors using histograms of height values, as they geometrically represent planar structures and can be represented by footprints, which commonly are constructed from closed contours formed by projecting wall segments onto horizontal planes. To ensure accurate footprint representation, non-wall objects, such as furniture, are first excluded from the scene. For this purpose, a series of viewpoints are used to simulate camera positions and generate image sequences. Coupled with these image sequences, a pretrained large-scale language-image model, YOLO-World, is applied to identify the bounding boxes of the furniture, while the SAM2 model is used to segment individual entities. The segmented pixels are then back-projected and aggregated in 3D space to isolate and exclude non-building objects. Once the walls are identified, the point clouds are processed using a region-growing and merging algorithm to extract multiple facades, which are projected onto horizontal planes to generate line segments. Based on these line segments and the scene’s bounding box, the horizontal plane is divided into cell partitions, and an energy optimization-based graph-cut algorithm is applied to identify the optimal cell set, with the resulting closed contours representing the footprints. These footprints are then extruded along the height direction into 3D geometries to generate Ifcwall, Ifcceiling, and Ifcfloor objects through the Ifcopenshell library, producing a complete and standardized IFC model.

This method was validated in complex indoor environments with furniture such as tables, chairs, and sofas, demonstrating high precision in reconstructing fundamental building components like walls, floors, and ceilings. By providing an automated and efficient solution for simple indoor structure reconstruction, the approach lays the groundwork for modeling more intricate scenarios and facilitates the development of intelligent, sustainable digital twin models to support comprehensive lifecycle building management.

How to cite: Zhai, R., Gan, X., He, Y., and Li, J.: Automated BIM Reconstruction from Point Clouds Using IFC Standards in Indoor Environment, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2727, https://doi.org/10.5194/egusphere-egu25-2727, 2025.

EGU25-3678 | ECS | Orals | GI5.2

NDT applied to monitor accelerated corrosion phenomena in engineering structures: a laboratory test with RC specimens 

Giuseppe Salvia, Davide Di Gennaro, Luigi Capozzoli, Emilia Vasanelli, Gregory De Martino, Stefania Imperatore, and Francesca Nerilli

Corrosion of reinforced concrete structures represents one of the main causes of degradation for civil structures and infrastructure, making the development of innovative strategies for monitoring their health strongly recommended. In this context, non-invasive geophysical methodologies have been demonstrated to be effective, but the information provided is often qualitative and not fully usable for engineering purposes [1-2].

A laboratory test was conducted at the Hydrogeosite CNR-IMAA facility to explore the potential of resistivity methods and electromagnetic techniques, aiming to uncover new relationships between signal variations and degradation phenomena.

Using an integrated approach, including Ground Penetration Radar (GPR), ultrasonic tests, and electrical techniques within the framework of the Icarus Project (PRIN Project 2022), a set of reinforced concrete samples was designed and subjected to accelerated corrosion tests in a saline solution. These samples are continuously monitored to identify corrosion phenomena in the rebar and degradation of the concrete.

The final goal of the test is to experimentally link bond-slip performance through the combined use of non-destructive testing (NDT) methodologies, supported by mechanical pull-out tests. This study highlights the pressing need to develop innovative strategies for monitoring the health of reinforced concrete structures, given the significant risks posed by corrosion. The integration of geophysical and non-destructive testing (NDT) methodologies forms the core of this research, aiming to bridge the gap between qualitative data and actionable engineering insights.

The methodologies developed in this study offer practical applications for assessing corrosion levels in reinforced concrete structures. The integration of geophysical and conventional NDT data provides an efficient, non-invasive approach for routine monitoring, which is particularly valuable for monitoring engineering structures.

Research activities are realized also exploiting instrumentations and facilities provided by the Research Infrastructures of IRPAC (Infrastruttura Tecnologica e di Ricerca per lo studio del passato umano, la Conservazione e Gestione del Patrimonio Culturale) and ITINERIS , Italian Integrated Environmental Research Infrastructures System).

 

References

Fornasari, G.; Capozzoli, L.; Rizzo, E. Combined GPR and Self-Potential Techniques for Monitoring Steel Rebar Corrosion in Reinforced Concrete Structures: A Laboratory Study. Remote Sens. 2023, 15, 2206. https://doi.org/10.3390/rs15082206

Capozzoli, L.; Fornasari, G.; Giampaolo, V.; De Martino, G.; Rizzo, E. Multi-Sensors Geophysical Monitoring for Reinforced Concrete Engineering Structures: A Laboratory Test. Sensors 2021, 21, 5565

How to cite: Salvia, G., Di Gennaro, D., Capozzoli, L., Vasanelli, E., De Martino, G., Imperatore, S., and Nerilli, F.: NDT applied to monitor accelerated corrosion phenomena in engineering structures: a laboratory test with RC specimens, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3678, https://doi.org/10.5194/egusphere-egu25-3678, 2025.

EGU25-4477 | ECS | Orals | GI5.2

Integrating Satellite Remote Sensing and Ethical AI for Cultural Heritage Preservation 

Tesfaye Tessema, Moein Motavallizadeh Naeini, Neda Azarmehr, Francesco Benedetto, and Fabio Tosti

Cultural heritage (CH) sites face escalating threats from environmental degradation, climate change, urbanization, and human activity. While traditional methods such as in-situ measurements and drone surveys using LiDAR and photogrammetry are valuable, they are often constrained by limited spatial coverage, revisit times, and operational challenges. To address these gaps, the integration of satellite remote sensing and artificial intelligence (AI) offers a transformative solution for scalable, continuous monitoring and automated change detection [1].

This study explores the combined use of multi-temporal satellite imagery—both optical and radar—and AI-driven algorithms to monitor structural changes and assess the environmental impacts on CH sites. By employing machine learning and deep learning models, the research enhances detection efficiency and accuracy, enabling non-invasive identification of structural deterioration, environmental stresses, and long-term degradation [2]. The approach emphasises using publicly available datasets and open-source tools to ensure accessibility and scalability.

In addition to technological advancements, the study adopts an ethical AI framework to address cultural and historical biases in CH monitoring. This framework seeks to minimise risks such as misrepresentation of marginalized communities and challenges posed by digitisation, including concerns about authenticity and the artificial reproduction of heritage assets. By integrating ethical considerations into the development and deployment of AI models, the research ensures that technological solutions align with sustainable and inclusive preservation practices.

The findings underscore the potential of combining advanced remote sensing technologies with AI to foster interdisciplinary collaboration, improve monitoring methodologies, and inform ethical policy frameworks. This integrated approach aims to safeguard cultural heritage sites for future generations.

 

Keywords: Cultural Heritage, Remote Sensing, Artificial Intelligence, Machine Learning, Monitoring

 

Acknowledgements

The Authors would like to express their sincere thanks and gratitude to the following trusts, charities, organisations and individuals for their generosity in supporting this project: Lord Faringdon Charitable Trust, The Schroder Foundation, Cazenove Charitable Trust, Ernest Cook Trust, Sir Henry Keswick, Ian Bond, P. F. Charitable Trust, Prospect Investment Management Limited, The Adrian Swire Charitable Trust, The John Swire 1989 Charitable Trust, The Sackler Trust, The Tanlaw Foundation, and The Wyfold Charitable Trust.

 

References

[1] Cuca, B., Zaina, F., & Tapete, D. (2023). Monitoring of Damages to Cultural Heritage across Europe Using Remote Sensing and Earth Observation: Assessment of Scientific and Grey Literature. Remote Sensing, 15(15), 3748.

[2] Argyrou, A., & Agapiou, A. (2022). A Review of Artificial Intelligence and Remote Sensing for Archaeological Research. Remote Sensing, 14(23), 6000.

How to cite: Tessema, T., Motavallizadeh Naeini, M., Azarmehr, N., Benedetto, F., and Tosti, F.: Integrating Satellite Remote Sensing and Ethical AI for Cultural Heritage Preservation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4477, https://doi.org/10.5194/egusphere-egu25-4477, 2025.

EGU25-6565 | Orals | GI5.2

Development of an integrated methodology for monitoring corrosion in reinforced concrete  

Enzo Rizzo, Federica Zanotto, Andrea Balbo, Fabio Menghini, Andrea Fabbri, and Vincenzo Grassi

In the context of degradation prevention and maintenance of civil infrastructure, there is a strong demand for non-destructive testing aimed at monitoring the condition of reinforced concrete systems, particularly regarding the corrosion of reinforcement bars. Rebar corrosion is one of the main causes of deterioration of engineering reinforced structures and this degradation phenomena reduces their service life and durability. Non-destructive testing and evaluation of the rebar corrosion by electrochemical tests is a major issue for predicting the service life of reinforced concrete structures. The research group of the University of Ferrara is gaining experience on this topic combining structural engineering and electrochemical techniques with NDT geophysical methods. The new regulatory provisions require the monitoring of "strategic" reinforced and prestressed concrete structures from the construction phase, conducting periodic investigations into reinforcement corrosion and maintaining a record of the data. Many non-destructive electrochemical techniques are useful for this purpose, such as measuring the open circuit potential (OCP) and linear polarization resistance (LPR), surface potential (SP) measurement, and measuring the resistivity of concrete. However, these methodologies are not so effective in the case of a structure where the degradation state is being assessed for the first time, because the electrochemical techniques allow for determining whether the corrosion process has initiated and estimate the corrosion rate at that time, but they are not able to assess the extent of degradation. Recently, Ground Penetrating Radar (GPR) has been applied to monitor the evolution of the corrosion process affecting reinforcement bars, also using new methods for processing GPR data, highlighting a strong correlation between the corrosive phenomenon and the electromagnetic response of the acquired signals. This project is proposing to develop an integrated methodology that enables the creation of a predictive model capable of estimating the overall degradation state of reinforced concrete and providing a quantitative assessment of its structural stability.

Over the past few years, numerous experiments have been conducted using various NDT methods, each capable of illustrating signal variations during the corrosion phenomena. These results emphasize the sensitivity of NDT methods in detecting rebar corrosion. The use of multi-sensor tools serves as the starting point for integrated observation, facilitating the transition from qualitative assessments to monitoring the evolving corrosion phenomenon on reinforced steel rebars. This approach aims to establish a quantitative analysis of the observed phenomena. For these aims, several reinforced concrete samples were produced using cement (Type II), suitable for structural applications, in which carbon steel rebars were embedded. The rebars were protected with an epoxy paint, leaving an exposed area of about 13 cm2. The samples were immersed in chloride-containing solutions and the rebars polarized for increasing periods of time. This aimed at inducing accelerated corrosion and achieving increased weight mass loss values of the exposed portion of the steel reinforcement. At the end of the polarization, the samples were opened for a degradation assessment and for actual mass loss evaluation. Finally the obtained weight loss values were correlated with the electromagnetic signals detected by GPR measurements.

How to cite: Rizzo, E., Zanotto, F., Balbo, A., Menghini, F., Fabbri, A., and Grassi, V.: Development of an integrated methodology for monitoring corrosion in reinforced concrete , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6565, https://doi.org/10.5194/egusphere-egu25-6565, 2025.

EGU25-6807 | ECS | Orals | GI5.2

Design of an Slotted Waveguide Antenna Array for Ground Controlled Interception (GCI) Radar 

Shailesh Pathak, Tannya Priya, and Amitabha Bhattacharya

This Abstract presents the design and analysis of an advanced Edge slotted waveguide antenna array tailored for high-gain applications within the S-band frequency range (2 GHz - 4 GHz). Initially developed for scientific and military purposes, slotted waveguide antennas (SWAs) have become a key component in various radar systems due to their exceptional features, including high directivity, low side lobe levels (SLL), low losses, excellent phase stability, and better power handling capabilities. The antenna array introduced in this work integrates as many as 40 number of radiating elements to achieve high gain and a sharply focused pencil-beam radiation pattern, making it ideal for radar and communication systems.


The radiating slots are precisely machined into the narrow wall of a WR-284 waveguide, ensuring both optimal electromagnetic performance and structural robustness. Comprehensive electromagnetic simulations confirm the antenna’s efficient operation within the S band, meeting the rigorous requirements of modern technologies. The design achieves a remarkable realized gain of 42.48 dBi, with beamwidths of 1.3° and 4.6° in the vertical and horizontal planes, respectively, and a VSWR of 1.24:1. The array , demonstrating the exceptional capabilities of slotted waveguide antennas in delivering high power, interference-resistant performance. These findings emphasize the critical role of SWAs in advancing radar and communication technologies.

How to cite: Pathak, S., Priya, T., and Bhattacharya, A.: Design of an Slotted Waveguide Antenna Array for Ground Controlled Interception (GCI) Radar, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6807, https://doi.org/10.5194/egusphere-egu25-6807, 2025.

EGU25-7714 | Posters on site | GI5.2

Verification of the accuracy of rock material determination by hammer strike sound using deep learning  

Daisuke Sugeta, Hirokazu Furuki, and Shigeru Miyamura

In geological fieldwork and concrete inspection, the sound of hammer blows is used to determine the quality of the material. In the case of rock, the sound of hammer blows is greatly influenced by the density of rock fractures and the heterogeneity of the rock composition. Therefore, even experienced geotechnical engineers may judge the goodness or badness of rock differently from person to person. Furthermore, the social issue of the lack of human resources of geotechnical engineers requires the application of new technologies, such as sensing technology and deep learning, to solve the problem.

In the field of civil engineering, deep learning technology is used to determine the state of deterioration from the sound of concrete being struck. However, rocks are more heterogeneous than concrete, and their applicability needs to be verified. In addition, there are no examples of matching technical decisions made by geotechnical engineers with deep learning models or verifying their accuracy. Therefore, in this study, a deep learning model was constructed based on spectral analysis of impact sound frequencies and learning audio information in order to quantitatively determine the material quality of rocks by impact sound. The validation target was rocks at a dam construction site in Japan.

The deep learning model employed a CNN, which has been reported to be used in a number of general audio classification problems, such as environmental sounds. Specifically, we constructed (1) YAMNET, which was transfer-trained on the impact sound of rock materials, and (2) 2D-CNN, which was trained by converting the impact sound of rock materials into log-mel spectrogram images, and conducted comparative verification. In order to construct the model, stratified 5-folds cross-validation was performed using data excluding test data, and optimal hyperparameters were searched.Also, the percentage of test data is 20% for all data.

As a result, we were able to construct a model with an F-score of approximately 90% with respect to the geotechnical engineer's judgement results. In the comparison between YAMNET and 2D-CNN, the F-score of 2D-CNN was superior by a few per cent. This difference can be attributed to the length of time of the input audio signal.

Finally, the model can estimate whether rock materials are good or bad with almost the same accuracy as a geotechnical engineer in the field. In addition, the deep learning model can make a decision in a few seconds. In the future we plan to make effective use of smartphones equipped with the model to improve the efficiency of field work and save manpower. In addition, validation will be carried out to estimate not only whether the rock material is good or bad, but also the detailed material classification. For the deep learning learning algorithm, we intend to compare and study state-of-the-art technologies, such as transformers, and to carry out verification to improve the accuracy of the system.

How to cite: Sugeta, D., Furuki, H., and Miyamura, S.: Verification of the accuracy of rock material determination by hammer strike sound using deep learning , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7714, https://doi.org/10.5194/egusphere-egu25-7714, 2025.

EGU25-8221 | Orals | GI5.2

3D Inversion of DCR Data for Structural Column Analysis in Buildings 

M. Emin Candansayar, Cansu Arıcan, and N. Yıldırım Gündoğdu

Geophysical methods have long been utilized for non-destructive testing of concrete structures, focusing on key techniques such as Ground Penetrating Radar (GPR), Direct Current Resistivity (DCR), and Seismic Methods (ultrasonic seismic). These methods assess factors like the condition of reinforcement bars, internal discontinuities, structural strength, and corrosion in concrete. In particular, DCR data, often collected with the Wenner array for fixed electrode distance, directly evaluates concrete corrosion through apparent resistivity. While some laboratory-scale resistivity tomography studies exist, this study introduces a novel measurement setup designed for multi-electrode and multi-channel DCR instruments. The setup enables data collection using different electrode arrays on building columns' single, adjacent, and opposite surfaces. We analyzed and compared the 3D inversion results obtained from synthetic and experimental data using various measurement setups and electrode arrays. This presentation will highlight the comparative results and insights gained from these configurations.

Acknowledgment: This study was supported by the Scientific and Technological Research Council of Türkiye (TÜBİTAK) under project ID 121Y281. We extend our sincere gratitude to TÜBİTAK for their valuable support.

 
 

How to cite: Candansayar, M. E., Arıcan, C., and Gündoğdu, N. Y.: 3D Inversion of DCR Data for Structural Column Analysis in Buildings, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8221, https://doi.org/10.5194/egusphere-egu25-8221, 2025.

EGU25-10960 | Orals | GI5.2

Challenges in Detecting Thin Asphalt Layers Using GPR 

Andreas Loizos, Christina Plati, and Alexandros Mouzakis

Ground Penetrating Radar (GPR) is a valuable tool in transportation infrastructure surveys that has evolved alongside the advancements in global technology. As a Non-Destructive Testing (NDT) technique, GPR is mainly utilized for pavement investigations and has been successfully used to assess the thickness in pavement engineering. However, despite its many years of use and improvements, there is still one major issue: how effectively can GPR detect thin asphalt layers? This challenge, commonly referred to as the "thin layer problem" according to the international literature, arises from the fact that it is difficult to detect reflections from thin layers. The main issue is the possible overlap of bottom and surface reflections, which makes accurate detection difficult.

The present research study addresses the accuracy requirements associated with using high frequency GPR antennas to identify and measure the thickness of thin asphalt layers. A key feature of this research is the proposed methodology, which provides a simple and effective approach to processing GPR data from thin asphalt layers to accurately detect their thickness. The methodology was validated using field data based on a highway section where rehabilitation works were carried out in conjunction with a newly constructed asphalt surface course. The estimated thickness of the thin layer showed an acceptable margin of error compared to the core sample measurements.

Overall, the results demonstrate the robustness and adaptability of GPR for quality assurance and quality control purposes, even in complex environments. In summary, GPR is a powerful tool that paves the way for more efficient pavement infrastructure management.

How to cite: Loizos, A., Plati, C., and Mouzakis, A.: Challenges in Detecting Thin Asphalt Layers Using GPR, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10960, https://doi.org/10.5194/egusphere-egu25-10960, 2025.

EGU25-14021 | Orals | GI5.2

Comprehensive Assessment of Asphalt Pavement Layer Compaction Degrees Using GPR-Based Density Profiling 

Siqi Wang, Yixiang Zhang, Tao Ma, Xiaoming Huang, and Guanglai Jin

Accurate assessment of asphalt layer compaction is crucial during the construction process. Ground-penetrating radar (GPR) technology allows continuous measurement of the dielectric constant of the surface layer, enabling comprehensive mapping of compaction levels. However, its application can be challenged by factors such as surface moisture resulting from roller nozzle sprays and the necessity of calibration coefficients in the dielectric constant-density relationship model. In this study, GPR technology was employed to develop an evaluation method for assessing the compaction quality of asphalt surface layers. Compaction metrics were analyzed by continuously collecting dielectric constant data from the asphalt surface layer, with the compaction interval and coefficient of variation used as indicators of compaction level and uniformity, respectively. The proposed method accounts for the impact of water vapor between the antenna and the ground on GPR accuracy and incorporates a data stability correction technique to remove outliers. The dielectric constant-density prediction model was calibrated through laboratory and field core testing. Field trial results demonstrate that GPR technology is effective in evaluating the compaction quality of asphalt layers. Unmanned compaction machinery was found to achieve better compaction uniformity, with a lower coefficient of variation compared to traditional methods. Variations in compaction were observed at the edges of construction sections and between lanes, showing the importance of improved construction monitoring to enhance overall compaction quality.

How to cite: Wang, S., Zhang, Y., Ma, T., Huang, X., and Jin, G.: Comprehensive Assessment of Asphalt Pavement Layer Compaction Degrees Using GPR-Based Density Profiling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14021, https://doi.org/10.5194/egusphere-egu25-14021, 2025.

EGU25-14087 | ECS | Orals | GI5.2

From Data to Decisions: Integrating Remote Sensing and a Reward and Benefit Analysis for Green Infrastructure Management 

Suman Kumari, Tesfaye Tessema, Laden Husamaldin, Parisa Saadati, Dale Mortimer, and Fabio Tosti

Sustainable Development Goal 3 of the 2030 Agenda for Sustainable Development is to “ensure healthy lives and promoting well-being for all at all ages”. Research consistently demonstrates that access to nature has profound benefits for physical health and mental well-being [1]. Green Infrastructure (GI), ranging from street trees, green roofs, parks, wildlife areas, woodlands, and wetlands, plays a vital role in supporting nature’s recovery, fostering biodiversity, and the ecosystem. Additionally, GI offers natural solutions to challenges like flood risk, poor air quality, and the urban heat effects exacerbated by climate change whilst creating inclusive spaces for people to experience physical and mental health benefits and delivering quality of life and environmental benefits for communities.

Recent studies show that urban green spaces alone support 2.1 million people to meet their weekly physical activities, estimated to be worth £5.6 billion, and reduce mental health service costs of approximately £141 million [2]. Acknowledging the critical role of GI for sustainable and resilient cities [3] and the challenges associated with an informed investment we propose the use of ‘reward and benefit’ analysis as an economic tool and utilization of medium-high-resolution remote sensing data and field information for mapping and monitoring of green infrastructures. Further, we propose to explore the correlation/link between the health impact of greener spaces on communities and the financial feasibility and viability of green spaces and projects.


Combining remote sensing and reward-benefit analysis creates a powerful framework for green infrastructure management and resilient urban development. Integration of spatial information and economic evaluations could support policy and decision-makers in evidence-based policy-plan development on prioritizing investments, resource allocation, enhanced stakeholder management, and healthier-happier neighbourhoods to achieve long-term sustainability goals.


Acknowledgments:
Sincere thanks to the following for their support: Lord Faringdon Charitable Trust, The Schroder Foundation, Cazenove Charitable Trust, Ernest Cook Trust, Sir Henry Keswick, Ian Bond, P. F. Charitable Trust, Prospect Investment Management Limited, The Adrian Swire Charitable Trust, The John Swire 1989 Charitable Trust, The Sackler Trust, The Tanlaw Foundation, and The Wyfold Charitable Trust.

References:
[1] Gunwoo Kim, Patrick A. Miller, The impact of green infrastructure on human health and well-being: The example of the Huckleberry Trail and the Heritage Community Park and Natural Area in Blacksburg, Virginia, Sustainable Cities and Society, Volume 48, 2019,101562, ISSN 2210-6707,(https://doi.org/10.1016/j.scs.2019.101562)

[2] Saraev, V., O’Brien, L., Valatin, G. and Bursnell, M. (2021), Valuing the mental health benefits of woodlands. Research Report. Forest Research, Edinburgh i-iv + 1-32pp

[3] Environmental Improvement Plan 2023 (https://www.nationalarchives.gov.uk/doc/open-government-licence/version/3/)

How to cite: Kumari, S., Tessema, T., Husamaldin, L., Saadati, P., Mortimer, D., and Tosti, F.: From Data to Decisions: Integrating Remote Sensing and a Reward and Benefit Analysis for Green Infrastructure Management, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14087, https://doi.org/10.5194/egusphere-egu25-14087, 2025.

EGU25-16105 | ECS | Posters on site | GI5.2

Retrieving signs of buried historical road tracks by GPR data processing 

Luca Bianchini Ciampoli, Saeed Parnow, Fabio Tosti, and Andrea Benedetto

Historic roads are integral to the cultural and visual heritage of landscapes, reflecting the historical narratives of regions and the populations they served. Mapping the planimetric and altimetric pathways of these ancient routes provides critical insights into how past societies interacted with their environment. Beyond their historical and archaeological value, rediscovered and restored roadways offer contemporary opportunities for "slow mobility," promoting sustainable tourism and local engagement with heritage sites [1].

This study presents a novel data-processing framework based on ground-penetrating radar (GPR) to improve the detection and geometric characterization of buried historical roads. The research focuses on two significant case studies in Rome, Italy-Villa dei Sette Bassi and Villa di Massenzio-where historical and archaeological evidence suggest the presence of uncharted ancient road connections.

The proposed methodology employs signal attribute-based analysis [2] to address key limitations in current detection techniques, including challenges posed by highly heterogeneous environments typical of archaeologically rich soils. By improving the accuracy and reliability of identifying structural components of ancient roadways, this approach advances our understanding of historical landscapes and supports sustainable heritage utilization strategies.

 

Acknowledgements

The authors would like to express their gratitude to the Parco Archeologico dell’Appia Antica and the Sovrintendenza Capitolina ai Beni Culturali for their support to the research and for providing access to the survey sites. Special thanks are also extended to Prof. Alessandra Ten, Prof. Carla Amici, and Dr. Ersilia Maria Loreti for their assistance with the archaeological interpretation.

How to cite: Bianchini Ciampoli, L., Parnow, S., Tosti, F., and Benedetto, A.: Retrieving signs of buried historical road tracks by GPR data processing, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16105, https://doi.org/10.5194/egusphere-egu25-16105, 2025.

EGU25-17586 | Posters on site | GI5.2

Conceptualization of toll road pavements assessment with non-destructive deflectometric testing  

Konstantinos Gkyrtis, Andreas Loizos, and Christina Plati

Toll pavements are an important part of highways, whose condition is not necessarily assessed according to strict monitoring procedures. So, they are almost overlooked when planning maintenance and rehabilitation measures. In addition, the particular nature of the concrete material typically used for toll plaza, makes it much more difficult to maintain healthy and functional structures. Examples of this include the propagation of cracks to full depth and more complex rehabilitation measures that require a complete replacement of the pavement slab, both of which are due to the brittle nature of concrete.

 

However, to ensure a resilient and sustainable road infrastructure, an accurate assessment of the condition of concrete pavements on site is crucial. Non-destructive testing enables non-invasive field inspections, and the Falling Weight Deflectometer (FWD) is the most convincing example of rapid defect detection and is a method that outperforms conventional core drilling. With this in mind, deflectometric testing was primarily used in this study to evaluate five toll plazas with in-service concrete pavements on a PPP highway for which no long-term monitoring data was available. A testing campaign was set up to evaluate the condition of each pavement slab or lane, assess the durability of the slabs, and determine the effectiveness of load transfer across joints and cracks.

 

The observed deflection variability of the slabs prompted a distribution fitting analysis to estimate characteristic values and thresholds for common deflectometric indicators, which were then verified against input data from pavement design. It is proposed to use the developed conceptual approach to establish evaluation criteria for individual slabs or damaged joints of concrete pavements, which could assist responsible decision makers in managing pavements and maximizing their resilience during their service life.

How to cite: Gkyrtis, K., Loizos, A., and Plati, C.: Conceptualization of toll road pavements assessment with non-destructive deflectometric testing , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17586, https://doi.org/10.5194/egusphere-egu25-17586, 2025.

EGU25-17848 | Orals | GI5.2

Structural Characterization of Infrastructures through multi-Methodological Geophysical Approach  

Vincenzo Serlenga, Maria Rosaria Gallipoli, Nicola Tragni, and Bojana Petrovic

As part of structural and infrastructure health monitoring, we propose a rapid and non-invasive experimental geophysical survey to determine the key structural parameters of an infrastructure. This approach involves the simultaneous acquisition of 20 minutes of seismic ambient noise using seismic arrays strategically placed at various points of the structure. These acquisitions do not require diverting or blocking traffic flow, nor does it disrupt the operation of road infrastructure.

The acquired signals are analyzed using various techniques, including standard spectral analysis (Fourier Amplitude Spectra, FAS), Frequency Domain Decomposition (FDD), Ambient Noise Deconvolution Seismic Interferometry (ANDI), and NonPaDAn analysis. This approach, which involves the joint application of these methods, was developed and validated on two types of viaducts: the Gravina Bridge, located on the SS.655-Bradanica, and the Monticello Viaduct on the SS.407-Basentana (Albano di Lucania), both in the Basilicata region of Italy.

The Gravina Bridge is a newly constructed arch bridge, and the structural parameters experimentally estimated are a reference point for future investigations into the evolution of these parameters over time. In contrast, the Monticello Bridge, a multi-span viaduct built in the 1970s, allowed for a comparison between the estimated structural parameters and the varying degrees of degradation observed in its girders.

By employing multiple analysis methods, the interpretation of results has been enhanced, demonstrating the potential of this approach to estimate the main vibrational modes, the relative modal shapes, equivalent damping, and seismic noise wave propagation velocities and the evolution of these parameters over time.

How to cite: Serlenga, V., Gallipoli, M. R., Tragni, N., and Petrovic, B.: Structural Characterization of Infrastructures through multi-Methodological Geophysical Approach , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17848, https://doi.org/10.5194/egusphere-egu25-17848, 2025.

EGU25-18307 | ECS | Orals | GI5.2

Road pavement conditions evaluation through NDT and BIM integration 

Luca Bertolini, Fabrizio D'Amico, and Luca Bianchini Ciampoli

Management and maintenance of transportation infrastructures are among the top priorities for public administrations and stakeholders around the world. Throughout the infrastructure lifecycle, data about asset conditions for all parties involved must be gathered and managed to develop strategies to reduce significant failures. Nowadays, there can be a lot of variation in the ways that different asset owners and contractors collect and handle data during a road's lifecycle. Due to the lack of a structured information system and information fragmentation, pavement management is vulnerable to significant rework, information loss, assessment errors, and misinterpretation of the collected data. Furthermore, a lot of issues with road pavements can arise in their deep layers, making it challenging to identify and examine them using conventional techniques. In this context, NDT methods, such as LiDAR and GPR, have been used alongside visual and automated testing to determine the root causes of pavement failures.

Building Information Modeling (BIM) can be a useful tool in this sense, providing an environment in which to store, manage and update data related to various infrastructure assets. In this context, the main goal of BIM integration in management procedures is to incorporate lifecycle data into digital three-dimensional models of the assets of civil infrastructures. Nonetheless, the road industry still lacks standardized processes for creating, integrating, representing, and maintaining data in BIM. This poses a problem for the industry, as there are currently no effective ways for the various disciplines and players involved in a road project to share data throughout its lifecycle.

The proposed methodology combines data provided by multiple NDT sources to generate a BIM model of a road pavement, that accurately depicts its configuration even regarding its deep layers. The digital representation of such an asset can be useful in carrying out analysis of its condition in a digital and three-dimensional environment. Moreover, pavement distresses found underneath the surface can be detected and integrated into the model, providing a more thorough and detailed representation of the pavement conditions. Using BIM procedures, such as clash detections methods, an automatic analysis of which pavement layers are affected by multiple kinds of distresses can be performed. Therefore, a database of pavement distresses, the corresponding layers and their location along the infrastructure can be obtained.

The methodology was tested on real data obtained during on-site surveys carried out on an Italian highway. The results show promising insight regarding the possible advancements in management and maintenance procedures of transportation infrastructures, as implementing BIM as a tool to store and manage information regarding pavement conditions can prove to be a great support to administrations and stakeholders in Italy and worldwide. Moreover, the use of the proposed process along the integrated analyses performed by IoT sensors, such in the case of bridges, can provide a more thorough insight regarding the entire infrastructure conditions, by comparing the ones related to its different assets.

Acknowledgements

This research is supported by the Projects “SIMICOM” accepted and funded by the Lazio Region, Italy (PR FESR Lazio 2021-2027 – "Riposizionamento Competitivo RSI")

How to cite: Bertolini, L., D'Amico, F., and Bianchini Ciampoli, L.: Road pavement conditions evaluation through NDT and BIM integration, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18307, https://doi.org/10.5194/egusphere-egu25-18307, 2025.

EGU25-18508 | Posters on site | GI5.2

IoT and BIM integrated platform for more efficient infrastructure monitoring and management 

Fabrizio D'Amico, Luca Bertolini, and Antonio Napolitano

Bridge monitoring and maintenance is renowned as a critical priority for governments and stakeholders 
worldwide. Such critical infrastructures play a fundamental role in transportation networks, therefore 
requiring constant monitoring to ensure a correct functioning of these networks, as well as the safety of 
road users. However, carrying out on-site surveys is usually time consuming, and funds are generally 
lacking, especially in the public sector. Therefore, methods to continuously obtain data regarding bridge 
conditions, while correctly storing and managing this information are required ever more by the industry.
Integration of Internet of Things (IoT) technologies into Building Information Modeling (BIM)
environments brings a new dimension to infrastructure monitoring and management by enabling realtime data acquisition, processing, and visualization procedures. Various IoT devices such as
accelerometers, temperature sensors, and environmental sensors can be used to supply the necessary 
stream of data continuously, thus creating a dynamic, holistic view of both structural and operational 
conditions of the analysed assets. All of these can also be integrated into BIM-based Digital Twin 
platforms for monitoring, and to predict needs in maintenance and lifecycle management.
This research addresses the methods for integrating IoT networks into BIM environments, creating an 
adaptive platform that could provide real-time updates and seamless data fusion. IoT sensors provide
localized and network-wide views of infrastructure conditions, including deformation patterns, thermal 
anomalies, and stress distributions. Synchronizing these data streams with BIM models gives 
stakeholders an intuitive and holistic platform for monitoring infrastructure health and planning 
interventions. Furthermore, the research delves into the challenges related to the integration of IoT and 
BIM, such as interoperability among diverse data sources, the continuous updating of BIM models, and 
the scalability of such systems for large-scale adoption. 
Applications using real world data show the potential of this approach in impacting the management of 
critical transportation assets such as bridges and viaducts. IoT-enhanced BIM systems are pathways to 
smarter, more resilient infrastructure networks by allowing proactive maintenance and efficient 
resource allocation. This research highlights the need for industry-wide collaboration in the 
standardization and adoption of such technologies so they can be effectively implemented at a global 
scale.
A

How to cite: D'Amico, F., Bertolini, L., and Napolitano, A.: IoT and BIM integrated platform for more efficient infrastructure monitoring and management, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18508, https://doi.org/10.5194/egusphere-egu25-18508, 2025.

EGU25-18888 | ECS | Orals | GI5.2

Ground Penetrating Radar and Community Engagement for Enhancing Resilience in Green Infrastructure  

Livia Lantini, Yasemin Didem Aktas, David Sanderson, Laden Husamaldin, and Parisa Saadati

As urban areas face increasing challenges from climate change, rapid urbanisation, and environmental degradation, enhancing urban resilience has become crucial for ensuring the sustainability of cities. Green infrastructure, particularly urban trees and green spaces, plays a central role in this effort, providing essential ecosystem services such as stormwater management, urban cooling, and carbon sequestration. However, the health and interaction of these natural systems with the built environment and infrastructure remain underexplored. Traditional methods for assessing the health of urban trees, particularly underground root systems, are often invasive and detrimental to the environment. This research explores the potential of non-destructive testing (NDT), specifically Ground Penetrating Radar (GPR), as a tool for assessing the health of urban trees and their underground root systems. 

This project aims to develop an innovative, non-invasive methodology using GPR to assess the underground root systems of urban trees and their interaction with infrastructure. By providing urban planners with accurate, actionable data, the project seeks to identify risks to both urban trees and surrounding infrastructure, thereby enhancing urban resilience. This research supports cities in managing green infrastructure more sustainably, promoting the integration of natural systems into urban planning, and helping cities become more adaptable to the challenges posed by climate change. 

The methodology involves using GPR technology to conduct surveys on urban tree root systems across various sites, mapping the underground root structures to identify potential risks to infrastructure, such as road damage or interference with utilities, and areas requiring preservation efforts. The GPR surveys are complemented by a review of tree species, urban settings, and environmental factors that impact root growth and health. A community-driven approach ensures that the data generated is applied in a way that directly benefits local communities, promoting collaborative solutions that integrate green infrastructure into urban planning. This approach aligns with the Sustainable Development Goals (SDGs), particularly SDG 11 (Sustainable Cities and Communities) and SDG 13 (Climate Action), by promoting climate-resilient urban environments through sustainable infrastructure practices. 

Preliminary results demonstrate the feasibility of using GPR as a non-invasive tool for enhancing resilience in urban planning. The research lays the foundation for developing a resilience framework to help cities integrate green infrastructure into climate adaptation strategies. This work will provide urban planners and policymakers with critical data for making informed decisions that strengthen the resilience of both urban ecosystems and infrastructure. 

Acknowledgements:  

This project is supported by the UK Department of Science, Innovation and Technology's International Science Partnerships Fund (ISPF) via the Royal Academy of Engineering under the Frontiers Seed funding scheme (FS-2425-22-157).

How to cite: Lantini, L., Aktas, Y. D., Sanderson, D., Husamaldin, L., and Saadati, P.: Ground Penetrating Radar and Community Engagement for Enhancing Resilience in Green Infrastructure , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18888, https://doi.org/10.5194/egusphere-egu25-18888, 2025.

EGU25-19401 | ECS | Orals | GI5.2

Advances, challenges and perspectives in fiber optic sensing applications to airport concrete pavement structural health monitoring 

Ruggero Pinto, Luca Bianchini Ciampoli, and Andrea Benedetto

Due to the recent awareness of climate change phenomena and ever-growing aircraft’s loads, superstructural health monitoring plays a pivotal role in effectively assessing an infrastructure’s degree of resilience. In this context, the contribution of non-destructive testing techniques - able to monitor structural conditions and survey extensive paved areas - needs to be reconsidered in favour of a potential synergy with real-time and pre-embedded monitoring sensors. By allowing seemingly continuous acquisition and immediate monitoring of strain and thermic pavement properties, fiber optic sensors’ applications could be deployed to measure rigid pavement behaviour and predict correspondent residual life. The present research focuses on the validation of such a technology through an ad hoc experimental setup, in order to assess the feasibility of an asset-wise, real-time data-driven concrete pavement management system. In conclusion, the encouraging outcomes of the experimental activities allow to consider the network of embedded structural health monitoring systems as an effective opportunity for managing extensive infrastructures, planning rehabilitation and maintenance strategies, ultimately preventing abrupt damage and unserviceability issues.

How to cite: Pinto, R., Bianchini Ciampoli, L., and Benedetto, A.: Advances, challenges and perspectives in fiber optic sensing applications to airport concrete pavement structural health monitoring, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19401, https://doi.org/10.5194/egusphere-egu25-19401, 2025.

EGU25-19747 | ECS | Posters on site | GI5.2

Non-Destructive Testing Approaches to Assess Water Ingress in Historic Masonry Ruins in the Context of Climate Change 

Nicoletta Bianchini, Efcharis Balodimou, Laden Husamaldin, Parisa Saadati, Tesfaye Tessema, Domenico D'Alessandro, and Fabio Tosti

Water is the main agent of deterioration in traditional buildings, particularly those with deficient or absent roofing and rainwater management systems. These sites wholly or partially surviving as ruins punctuate and define the landscape and represent invaluable heritage assets at risk of deterioration [1, 2].

In this research, the authors focus on historic masonry ruined structures located in England. An extensive literature review is used to investigate deterioration mechanisms and the role of climate change [3, 4], identify recurrent causes and sources of water ingress, evaluate the role of vegetations as well as the role of different maintenance regimes and past interventions.

The project will also investigate the most appropriate non-destructive testing (NDT) methods able to monitor and develop easy and repeatable methods of water ingress assessment in historic masonry ruined structures [5, 6]. The study focuses on the use of popular (e.g., ultrasound, ground-penetrating radar (GPR)) and less conventional NDTs in this domain, understanding main capabilities and limitations. The methods can set competencies, recurrent locations along the structure, accessibility and principles to underpin investigation and treatment of water ingress in traditional buildings. The paper concludes with recommendations for future research in this area. It includes the implementation of the most advanced non-destructive testing techniques and the acquisition of additional data concerning the behaviour of masonry structures under varying environmental conditions.

 

Keywords: Historic Masonry Ruins, Roofless Structures, Non-destructive Testing (NDT), Water Ingress, Climate Change

 

Funding: This is part of a Historic England funded project with title: “Collapse of Masonry Walls in Historic Ruined Structures: Understanding the Underlying Causes and Warning Signs; Identifying Investigation Strategy and Preventive Conservation Measures”.

 

References

[1] Ramirez, Ghiassi, Pineda and Lourenço, “Moisture and Temperature Effects on Masonry Structures: The Civic Tower of Pavia as a Case Study,” Lect. Notes Civ. Eng.

[2] Sass, O. & Viles, H. Heritage hydrology: a conceptual framework for understanding water fluxes and storage in built and rock-hewn heritage, Heritage Sci.

[3] Tolley, “Wigmore Castle, Herefordshire, the repair of a major monument: an alternative approach.”

[4] Laycock and Wood, “Understanding and controlling the ingress of driven rain through exposed, solid wall masonry structures,” Geol. Soc. Spec. Publ.,

[5] Franzoni, Berk, Bassi and Marrone, “An integrated approach to the monitoring of rising damp in historic brick masonry,” Constr. Build. Mater.

[6] M.I. Martinez-Garrido, R. Fort, M. Gomez-Heras, J. Valles-Iriso, M.J. Varas-Muriel, “A comprehensive study for moisture control in cultural heritage using non-destructive techniques, J. Appl. Geophysics.

How to cite: Bianchini, N., Balodimou, E., Husamaldin, L., Saadati, P., Tessema, T., D'Alessandro, D., and Tosti, F.: Non-Destructive Testing Approaches to Assess Water Ingress in Historic Masonry Ruins in the Context of Climate Change, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19747, https://doi.org/10.5194/egusphere-egu25-19747, 2025.

EGU25-20016 | ECS | Orals | GI5.2

Digital Twin for Advanced and Continuous Monitoring of Infrastructure Assets Using Remote Sensing and Non-Destructive Testing 

Antonio Napolitano, Valerio Gagliardi, Alessandro Calvi, Jhon Rome Diezmos Manalo, and Andrea Benedetto

The structural integrity of transportation infrastructure is critical in ensuring public safety, economic stability and societal advancement. The demand for versatile, scalable and real-time monitoring solutions becomes exponential as these assets age, get used more and face environmental pressures. Conventional inspection methods, such as visual inspections and static evaluations, while valuable in localized applications, have significant limitations, including dependence on the expertise of specialized operators, time consumption, and an inability to provide dynamic insights across extensive networks [1]. In this regard, Digital Twin (DT) technology has emerged to provide a virtual replica of physical assets in real-time with data from multiple sources [2]. Supplementing DTs, remote sensing techniques including Multi-Temporal InSAR (MT-InSAR) and high-resolution satellite images can easily identify structural displacements in the millimeter scale region over extensive region.

Satellite constellations, provide periodical updates with high spatial and temporal resolution, allowing a near real time monitoring of infrastructure without the need for ground-based instrumentation. These advancements are further enhanced by Building Information Modeling (BIM), which supports the creation of dynamic digital models encompassing all data relevant to the management, maintenance, and optimization of transportation infrastructure. This research presents a comprehensive approach to integrating Digital Twin technology with satellite remote sensing, BIM, and non-destructive testing methodologies. The study highlights the potential of combining near-real-time satellite data, field inspections, and advanced visualization techniques to develop a scalable, network-level monitoring system for critical assets such as bridges and viaducts. These results reiterate the value of high-resolution satellite missions along with next-generation technologies for enabled predictive maintenance and structural integrity management, supporting the sustainable and resilient transportation infrastructure development.

 

Acknowledgements

This research is supported by the Project “PIASTRE” accepted and funded by the Lazio Region, Italy

References

[1] Napolitano A., et al., Integration of Satellite Monitoring data in a Digital Twin of Transport Infrastructure. Proceedings Volume 13197, Earth Resources and Environmental Remote Sensing/GIS Applications XV; 131970Y (2024) https://doi.org/10.1117/12.3034395

 

[2] Gagliardi V., et al., Digital twin implementation by multisensors data for smart evaluation of transport infrastructure. SPIE Optical Metrology. Multimodal Sensing and Artificial Intelligence: Technologies and Applications III, Munich, 2023.

How to cite: Napolitano, A., Gagliardi, V., Calvi, A., Manalo, J. R. D., and Benedetto, A.: Digital Twin for Advanced and Continuous Monitoring of Infrastructure Assets Using Remote Sensing and Non-Destructive Testing, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20016, https://doi.org/10.5194/egusphere-egu25-20016, 2025.

EGU25-20180 | Orals | GI5.2

Enhanced Deformation Monitoring in Virtual Reality using Remote Sensing Data in Airport Runway Management 

Stephen Uzor, Elikem Atsakpo, Tesfaye Tessema, Luca Bianchini Ciampoli, Valerio Gagliardi, Andrea Benedetto, and Fabio Tosti

Deformation monitoring in airport runways is a key task in airport management and operations requiring prompt intervention and actions to maintain surface regularity. The technological advancement in this area has been dramatic. Terrestrial and aerial remote sensing can provide accurate and dense deformation data [1]. In the past decade, the use of satellite observations for airport monitoring has grown due to the advantage of accurate results with high temporal and spatial resolution [2]. However, the satellite remote sensing data are still deployed conventionally to users through bi-dimensional maps and charts, therefore limiting the level of interaction of end-users and impacting the decision-making process. Immersive technologies can fill this gap [3] by enhancing the visualization and communication of information from satellites in spatial environments [4], enabling a better understanding of surface deformations in runways.

This research explores the design of a Virtual Reality (VR) tool for visualizing multi-temporal deformations at Runway 3 of the ‘Leonardo Da Vinci Airport’ in Fiumicino, Rome, Italy. The protocol encompasses the use of high-resolution data acquired during November 2016 to December 2019 and processed using the Permanent Scatterer Interferometry (PSI) technique. The tool is developed in Unity 3D with the following key design goals:

  • Cross-validation with two or more VR headsets allowing for multi-user collaborative analysis.
  • 3-dimensional interactive visualizations that allow for scalability in visualizing data at the millimeter level as well as isolating sections of interest to stakeholders.
  • Analysis of historical structural data using machine learning to predict future deformations and highlight potential risks.

Using satellite remote sensing, we combined sub-millimeter information on the displacements of the pavement runway with the total station to provide a holistic digital model of the physical site. The system can provide an efficient infrastructure modelling and assessment solution, which will allow researchers and engineering professionals to a) create digital 3D snapshots of a physical site for later assessment, b) track positional data on existing displacements, and c) inform the decision-making process regarding locations for early and potential future interventions.

 

References

[1] Bianchini Ciampoli et al. Displacement Monitoring in Airport Runways by Persistent Scatterers SAR Interferometry. Remote Sensing. 2020; 12(21):3564.

[2] Gagliardi, et al. Testing Sentinel-1 SAR Interferometry Data for Airport Runway Monitoring: A Geostatistical Analysis. Sensors. 2021; 21(17):5769.

[3] Wang, Peng, et al. “A Critical Review of the Use of Virtual Reality in Construction Engineering Education and Training.” International Journal of Environmental Research and Public Health, vol. 15, no. 6, June 2018, p. 1204.

[4] Luleci, Furkan, et al. “Structural Health Monitoring of a Foot Bridge in Virtual Reality Environment.” Procedia Structural Integrity, vol. 37, 2022, pp. 65–72.

Acknowledgments: Sincere thanks to the following for their support: Lord Faringdon Charitable Trust, The Schroder Foundation, Cazenove Charitable Trust, Ernest Cook Trust, Sir Henry Keswick, Ian Bond, P. F. Charitable Trust, Prospect Investment Management Limited, The Adrian Swire Charitable Trust, The John Swire 1989 Charitable Trust, The Sackler Trust, The Tanlaw Foundation, and The Wyfold Charitable Trust. 

How to cite: Uzor, S., Atsakpo, E., Tessema, T., Bianchini Ciampoli, L., Gagliardi, V., Benedetto, A., and Tosti, F.: Enhanced Deformation Monitoring in Virtual Reality using Remote Sensing Data in Airport Runway Management, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20180, https://doi.org/10.5194/egusphere-egu25-20180, 2025.

After 20 years, with 12,854 ± 0.056 ka BP (Wolbach,2018) YDIH, Younger Dryas Impact Hypothesis (Firestone,2007,2009; Moore,2024) confirmed original date of 12.850 cal yrs BP for Continental-Ice, CI-KISS (Bujatti-Narbeshuber,1997b).

270 yrs earlier, Mayan Codex Troano date of Atlantic-Ocean, AO-KISS (13.124 BP), corroborated by Laacher See Eruption (LSE) as impact-volcanism proxy date (Bujatti-Narbeshuber,1997), now 13.160 (Friedrich,2004;Kromer,2004), 13.034 yrs BP (Van Raden,2019), is expanded by Greenland bipolar sulfate (Lin,2022) as Impact-Volcanism-Quadruplet (IVQ). LSE marks start of 5 step-geomagnetism (Dichiara,2023) and (Gravity-Greenhouse Threshold Transition) GTT2-warming “staircase” where LSE-IVQ cooling is overwhelmed by H20-gravity-warming (Nikolov,2024,Jucker,2024). GTT2 characterizes Inter-Aleroed-Cold-Period 2 (IACP2) reaching its maximum with Holocene-End-Aleroed-Temperature (HEAT) Melt-Water-Pulse (MWP) 0B with < 6m step in sea level (Bard,2010), the real Younger-Dryas- Onset (YDO) trigger, years later reinforced by CI-KISS (12,854 ka BP), supporting biphasic YD-cooling (Max,2022), then warming MWP1B.

IACP evolves through Atlantic-Ocean (AO-) KISS with Mid-Atlantic Ridge & Plateau Lowering Events (MARPLEs), meso-stratospheric water and gas plume of 25,03 x 1015  tons (Muck,1976), first into IAPC1-Albedo cooling phase (Repschläger,2023) with bleached magmatic, silico-clastic (Davias and Gilbride,2012) “White Mats” (Bujatti-Narbeshuber,2023) and geomagnetic (Mörner,1977; Chen,2020) Gothenburg-Excursion-Onset (GEO), later LSE, marks, despite 5 LSE-IVQ volcanic cooling episodes, the restart into IAPC2 with the rewarming Gravity-Greenhouse-Threshold GTT-staircase.

Finally the full, both Continental-Ice and Atlantic-Ocean (CIAO-) KISS scenario (Bujatti-Narbeshuber and Hoogewerff,1995), is necessary to explain and predict Pleistocene/Holocene-Catastrophic-Climate-Change (PHCCC).

Research on PHCCC starts from the hypothesis that a Koefels-comet Taurid-fragment impacted into the Ötztal glacier ice near Hohe Geige mountain (3393 m, Tirol, Austria) with Pleistocene/Holocene KISS serving as long sought, necessary trigger factor for the pre-failure weakening of the Koefels crystalline rock, “since there is no other evidence for a pre-existing zone of weakness promoting slope failure” (Zangerl,2021).

Holocene retreat of stabilizing ice, much later, around 9527-9498 cal BP (Nicolussi,2015), lead to the extremely rapid rock slide of Koefels with 3,28 km3 (Brückl,2001).

Koefels-crater is the largest crater in the metamorphic, crystalline area of the Alps. Even seismic fatigue cannot solely explain (Oswald,2021) without the KISS-impact “the particular situation of the Koefels rockslide because it is still unclear why this giant event occurred at this location and within a very strong rock mass” (Zangerl,2021).

Hohe Geige and Koefels crater are furthermore positioned above a unique circular Geomagnetic Anomaly (Ahl, Slapansky,2003) evident in the aeromagnetic map of Austria (Seiberl,1991), suggested  as impact magnetism based on growing evidence for a global CIAO-KISS event (Bujatti-Narbeshuber,1997a).  

Hohe Geige and Koefels extend northward into a sector, widening from 12 to 17 km, 50 km long, that contains the largest concentration of rock slides (12) in the Alps (Tollmann,1992; Abele,1974). This is explained by both seismicity or an ejecta curtain from an oblique KISS-impact and already led to solving the Carolina Bays enigma as late Pleistocene, 12.850 cal yrs BP, “paleoseismic, impact-seismic, liquefaction features” (Bujatti-Narbeshuber, 1997b).

Koefels-comet Taurid-fragments with an oblique Ice-impact into the Ötztal glacier low-impedance ice-layer “guiding the pressure wave horizontally thus absorbing up to 70% of the impact energy would significantly reduce both the peak pressures at depth along with their expressions in the rock record” (Stickle,Schultz,2012,2013; French, Koeberl,2010).

How to cite: Bujatti-Narbeshuber, M.: Pleistocene/Holocene (P/H) boundary oceanic Koefels-comet Impact Series Scenario (KISS) of 12.850 yrs BP Global-warming Threshold Triad (GTT): Part V, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20574, https://doi.org/10.5194/egusphere-egu25-20574, 2025.

Void defects significantly undermine the safety and operational performance of ballastless tracks in high-speed railways [1]. Ground Penetrating Radar (GPR), serving as a non-destructive testing tool, is widely used for detecting internal defects in ballastless tracks, owing to its fast detection speed and high resolution. However, the complex rebar distribution in track slabs causes severe interference in GPR data during detection, reducing the detectability of void signals, while the sensitivity of GPR data to void defects detection varies across different polarization modes, further complicating accurate identification [2].

To address these challenges, this paper proposes a void defects detection method by rebar clutter suppression and polarization fusion imaging. First, a deep learning model is developed to suppress rebar clutter in GPR data, improving void signal visibility. Then, Reverse Time Migration (RTM) is applied to fuse data from HH and VV polarization modes, further enhancing imaging resolution and accuracy [3].

The proposed method is validated through forward modeling and field experiments. Results demonstrate its effectiveness in suppressing rebar clutter and improving void detection and imaging. This paper provides an approach for structural health monitoring of ballastless tracks, offers insights into advancing GPR applications in complex rebar environments, and introduces a new perspective for using GPR in the detection of ballastless tracks.

References:

[1] Yang, Y., & Zhao, W. (2019). Curvelet transform‐based identification of void diseases in ballastless track by ground‐penetrating radar. Structural Control and Health Monitoring, 26(4), e2322.

[2] Wang, X., Liu, H., Meng, X., Cui, J., & Du, Y. (2024). Enhanced imaging of concealed defects behind concrete linings using Residual Channel attention network for rebar clutter suppression. Automation in Construction, 166, 105574.

[3] Liu, H., Yue, Y., Lian, Y., Meng, X., Du, Y., & Cui, J. (2024). Reverse-time migration of GPR data for imaging cavities behind a reinforced shield tunnel. Tunnelling and Underground Space Technology, 146, 105649.

How to cite: Peng, H. and Liu, H.: Rebar Clutter Suppression and Fusion Imaging for Enhanced Detection of Void Defects in Ballastless Tracks Using Ground Penetrating Radar, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20939, https://doi.org/10.5194/egusphere-egu25-20939, 2025.

EGU25-21012 | ECS | Orals | GI5.2

Advanced monitoring of road pavement and infrastructure degradation using mobile laser scanning and ground penetrating radar 

Alessandro Di Benedetto, Andrea Benedetto, Luca Bianchini Ciampoli, Margherita Fiani, David Loncarevic, Antonio Luca Morabito, and Luigi Petti

The primary objective of this study is to develop efficient surveying and data processing methodologies that enable the extraction of more detailed metric data on road infrastructure than what can be obtained through traditional survey techniques.

Condition assessments conducted using traditional methodologies may be risky and, in some cases, ineffective. The Mobile Laser Scanner (MLS) technique, based on LiDAR technology, is widely adopted as a reliable alternative, as it allows for the generation of dense, accurate point clouds of both the road surface and associated artworks.

The aim of our work is to provide a comprehensive workflow for processing MLS data to generate useful indicators that describe the functional and structural characteristics of both the pavement and related structures, with the goal of optimizing decision-making processes for infrastructure managers.

Data processing for road surface analysis involves three main stages: (i) Extraction of points corresponding to the road pavement or the surfaces of associated structures; (ii) Generation of a curvilinear abscissa Digital Elevation Model (DEMc); and (iii) Analysis of surface regularity and the intrados of the artworks.

Point cloud filtering relies on the M-estimator SAmple Consensus (MSAC) algorithm, a robust variant of the RANSAC method. The DEMc is designed to follow the curvilinear alignment of the road axis. A curvilinear planimetric grid is first generated, with the curvilinear abscissa corresponding to the points marked by horizontal road signage. Elevation values are then assigned to each grid node, derived via local interpolation of points from the road surface. Surface condition assessment and cross-slope analysis are conducted by examining each cross-profile extracted from the DEMc. For each profile, regularity indices such as Rut Depth, as well as characteristic geometric parameters like transverse slopes, are calculated.

Regarding the analysis of structures, particularly tunnel intrados, our study proposes a methodology that utilizes an automatic unrolling algorithm for point clouds of the intrados, based on the RANSAC method. Intensity values of the LiDAR data are then analyzed to detect potential water infiltrations, while roughness values are calculated to assess surface integrity and identify cracks or steel bar ejections. The results, though focused on only two types of degradation, are useful for pinpointing tunnel sections in need of urgent intervention, thereby indicating areas of high priority for action or alert. The entire process is implemented in MATLAB.

The condition of the underlying layers of the road pavement were examined through Ground-Penetrating Radar (GPR) measurements to identify potential damage sources responsible for the deterioration of the surface layers. This also enables an assessment of whether the deformations affect only the superficial layers or extend to deeper strata. The outcome of the entire process is the creation of an Atlas in QGIS.

Data acquisition was carried out using a Leica Pegasus TRK500 Neo MLS, in collaboration with C.U.G.RI., Leica Geosystems for the survey, and SPN Salerno Pompei Napoli S.p.A. for logistical support. The survey was conducted over a 4 km stretch of the A3 highway (Campania Region, Italy), an area significantly affected by hydrogeological hazard.

How to cite: Di Benedetto, A., Benedetto, A., Bianchini Ciampoli, L., Fiani, M., Loncarevic, D., Morabito, A. L., and Petti, L.: Advanced monitoring of road pavement and infrastructure degradation using mobile laser scanning and ground penetrating radar, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21012, https://doi.org/10.5194/egusphere-egu25-21012, 2025.

EGU25-21016 | Posters on site | GI5.2

An integrated structural model for predicting rigid pavement damage based on NDT survey data 

Andrea Benedetto, Ruggero Pinto, Luca Bianchini Ciampoli, and Valerio Vezzari

Designed to withstand repetitive cycles of aircrafts’ static loads and thermic gradients, apron rigid pavement requires long-term serviceability and structural reliability throughout its service period. Due to the vast dimensions of concrete superstructural asset monitored, international and local aviation regulative agencies advise the implementation of an effective Airport Pavement Management System (APMS), leading to structural analysis and residual service life prediction models of the existing asset to support airport handlers in construction and maintenance strategies.
Relying on measuring paved areas’ evolutive conditions, in an APMS it is recommended to carry out space and time consistent multi-source Non-Destructive Testing techniques (NDT). At the present state-of-the-art geometrical and mechanical properties collected through NDT surveys are individually analysed and compared against correspondent alarm thresholds. The disaggregated elastic and structural information from each NDT technique conveys into a pavement mechanics analysis, usually performed through finite element methods at the scale of sample unit of measurement. The resultant stress field for the specific superstructural configuration feeds a cumulative concrete fatigue damage and residual life model based on sample unit’s preset service period and traffic mix.
To accurately estimate priority of intervention assessing functional entity, degrading condition severity and asset importance, a structural model for rigid pavement elastic analysis based on NDT survey data needs to be further refined at the level of detail of each elementary unit surveyed. By using the same level of detail of NDT data collection stage, an analytical approximate solution for rigid mechanic and thermic rigid pavement rheological behaviour is being developed as an interoperable and computationally efficient alternative to finite element methods. Conveying NDT sampled properties for each elementary unit into a related structural and damage analysis, an effective pavement management system could be achieved for data-driven and airport-wise scalable asset management.

How to cite: Benedetto, A., Pinto, R., Bianchini Ciampoli, L., and Vezzari, V.: An integrated structural model for predicting rigid pavement damage based on NDT survey data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21016, https://doi.org/10.5194/egusphere-egu25-21016, 2025.

EGU25-971 | ECS | Posters on site | GI5.3

Uncertainty maps as a tool for efficient AUV data collection 

Ana Filipa Duarte, Lucrezia Bernacchi, Renato Mendes, João Borges de Sousa, and Leonardo Azevedo

Autonomous Underwater Vehicle (AUV) trajectory planning for oceanographic surveys should ensure comprehensive data collection for enhanced mission success. By strategically navigating and targeting high-value data points, the AUV can operate longer and gather more essential information for ocean modelling. Here, we propose a geostatistical modelling workflow to predict ocean temperature with spatial uncertainty maps, representing regions with limited knowledge about the ocean properties from where navigation paths can be devised.

A real autonomous oceanographic survey performed off W. Portugal illustrates the proposed modelling workflow. To spatially predict ocean temperature and uncertainty for the ‘day after’, we use Direct Sequential Simulation[1]. We also use the CMEMS[2] product of Atlantic-Iberian Biscay Irish- Ocean Physics Analysis and Forecast as experimental data to constrain the spatial predictions. During the survey, the daily updated numerical ocean model is downloaded to accommodate new information, and the AUV data is assimilated and used in new geostatistical predictions.

At the beginning of the survey, we predict the ‘day after’ based on the previous 14 days, a spatiotemporal covariance matrix and the CMEMS[2] product as experimental data without uncertainty. The pointwise median model of an ensemble of geostatistical realizations is used as the most likely model, while the pointwise standard deviation model is used as an uncertainty measurement. This uncertainty map is used to devise the navigation strategy using a prize-collecting vehicle routing problem solver. At the end of each day, the data acquired by the AUV is assimilated to contain the prediction of the ocean temperature for the following day along with the updated CMEMS[2] ocean model.

The results show that the proposed methodology efficiently predicts daily ocean temperature and its spatial uncertainty and assimilates data from different sources. The AUV was able to sample ocean regions associated with higher uncertainty (i.e., variability).

References

[1] Soares, A., 2001, Direct sequential simulation and cosimulation: Mathematical Geology, 33, 911–926, doi: 10.1023/A:1012246006212.                          

[2] Atlantic-Iberian Biscay Irish- Ocean Physics Analysis and Forecast. E.U. Copernicus Marine Service Information (CMEMS). Marine Data Store (MDS). DOI: 10.48670/moi-00027 (Accessed between 14 to 25-Oct-2024)

How to cite: Duarte, A. F., Bernacchi, L., Mendes, R., Borges de Sousa, J., and Azevedo, L.: Uncertainty maps as a tool for efficient AUV data collection, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-971, https://doi.org/10.5194/egusphere-egu25-971, 2025.

EGU25-1089 | ECS | Posters on site | GI5.3

Mapping Soil Porosity: Unveiling India's Soil Dynamics with Remote Sensing 

Harshita Rani Ahirwar, Ashish Pratap Singh, Manish Kumar Nema, and Anupam Kumar Nema

The physical state of the soil environment majorly defines plant growth.  The composition and properties of the soil matrix influence various transport processes and important flow between soil and plant. The porosity and density of soil help determine the water binding possibility, air movement, plant root penetration, etc. Just as the solid phase the geometry of the pore system is also complex. The porosity of the soil matrix is determined using densities- particle density and bulk density.  On the one side where we have several methods to determine porosity, we lack in the spatial details of it. Many attempts have been made to gather information about porosity through machine learning and remote sensing methods for specific locations. The present study attempts to map the porosity details over India using various databases and finally checking the accuracy and reliability of data sources.

How to cite: Ahirwar, H. R., Singh, A. P., Nema, M. K., and Nema, A. K.: Mapping Soil Porosity: Unveiling India's Soil Dynamics with Remote Sensing, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1089, https://doi.org/10.5194/egusphere-egu25-1089, 2025.

EGU25-3548 | Posters on site | GI5.3

Low-Frequency Ground Penetrating Radar: A Versatile Tool for Multiscale Analysis in Active Tectonics, Geoarchaeology, and Urban Geology 

Bruno Massa, Nicola Angelo Famiglietti, Antonino Memmolo, Robert Migliazza, and Annamaria Vicari

In situ geophysical techniques are essential tools in geological and geotechnical research for characterizing tectono-stratigraphic settings. Since its introduction in the late 1970s, Ground Penetrating Radar (GPR) provides integrated information over a large subsoil volume, overcoming the limitations of conventional point-scale direct survey or measurements. In the last decade, advances in low-frequency GPR systems have made them efficient and affordable for multiscale investigations. Compact and lightweight monostatic antennas, such as the COBRA Plug-In SE 70 employed in this study, allow for rapid deployment, flexible parameter settings, and high-resolution data acquisition. Operating with a center frequency of 80 MHz, a frequency range of 20–140 MHz, and a maximum penetration depth of 50 meters, this system achieves vertical resolutions of approximately 30 cm with a sampling rate of 32,000 sample/s. This study presents the results of low-frequency GPR surveys conducted in different geological contexts in Southern Italy:1) active tectonics at Mt. Camposauro (Southern Apennine, Italy) an area of energetic historical seismicity with evidences of recent tectonic activity; 2) geoarchaeology and site characterization of subsurface caves at the ancient Capua, an Etruscan city (IX century BCE) lately conquered by  Osci, then by Samnite (IV century BCE) and finally by Romans, becoming in the III century BCE the main city along the Via Appia, regina viarum;  and 3) urban geology in Calitri Town (Avellino, Italy) an area with a complex tectono-stratigraphic setting, affected by seismically induced gravity-driven deformations. The results highlight the versatility and effectiveness of low-frequency GPR for investigating geological processes at varying spatial and temporal scales. Key findings are summarized and discussed, emphasizing the role of GPR as a preferred method for integrated subsurface analysis.

How to cite: Massa, B., Famiglietti, N. A., Memmolo, A., Migliazza, R., and Vicari, A.: Low-Frequency Ground Penetrating Radar: A Versatile Tool for Multiscale Analysis in Active Tectonics, Geoarchaeology, and Urban Geology, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3548, https://doi.org/10.5194/egusphere-egu25-3548, 2025.

EGU25-4629 | ECS | Posters on site | GI5.3

Seismic monitoring experiment of deep-sea driling 

yunlong liu, lei qiu, hanchuang wang, and chunhui tao

As human exploration and exploitation of seabed mineral resources intensify, concerns about the degradation of the ocean bottom noise environment have risen. To address this, we conducted a seismic monitoring experiment during the 78th Chinese Dayang cruise in 2023, focusing on drilling activities at the Yuhuang seafloor massive sulfide deposits located at the Southwest Indian Ridge. Five Ocean Bottom Nodes (OBNs), each equipped with three orthogonal seismometers and one hydrophone operating at a sampling rate of 1000 Hz, were deployed around a sulfide mound by using the "Hailong IVE" ROV, which featured a real-time Ultra-Short Baseline (USBL) positioning system for precise placement. Additionally, high-sampling-rate cabled hydrophones, capable of capturing data at 32 kHz, were installed on a cable positioned 15 meters above the seabed drill site. Throughout the experiment, a seabed drilling rig capable of drilling up to 20 meters below the seafloor conducted a total of 13 drill operations. Our objectives were to identify drilling-related signals from the seawater and drill bit signals from the subseafloor, assess the impact of drilling operations on marine noise, and invert the velocity structure using ambient noise data. The initial insights gained from our experiment indicate that the maximum radius of drilling-related noise does not exceed 100 meters. The noise level produced by the drilling rig is influenced by the drilling parameters, such as revolutions per minute and weight on bit, as well as the hardness of the rock. To gain a more comprehensive understanding of the impact of drilling activities on the ocean sound field, further drilling tests with additional seismometers and hydrophones are necessary. This will provide a richer dataset, enabling more accurate assessments of noise generation and propagation patterns associated with seabed drilling operations.

How to cite: liu, Y., qiu, L., wang, H., and tao, C.: Seismic monitoring experiment of deep-sea driling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4629, https://doi.org/10.5194/egusphere-egu25-4629, 2025.

EGU25-5448 | ECS | Orals | GI5.3

DC_OCEAN: An open-source algorithm for identification of duplicates in ocean databases 

Xinyi Song, Zhetao Tan, Ricardo Locarnini, Simona Simoncelli, Rebecca Cowley, Shoichi Kizu, Tim Boyer, Franco Reseghetti, Guilherme Castelao, Viktor Gouretski, and Lijing Cheng

A high-quality hydrographic observational database is essential for ocean and climate studies and operational applications. Because there are numerous global and regional ocean databases, duplicate data continues to be an issue in data management, data processing and database merging, posing a challenge on effectively and accurately using oceanographic data to derive robust statistics and reliable data products. This study aims to provide an algorithm to identify the duplicates and assign labels to them. We propose first the definition of exact duplicates and possible duplicates; and second, an open-source and semi-automatic system (named DC_OCEAN) based on crude screening and target screening, which is followed by a manual expert check to review the identified duplicates to detect duplicate data and erroneous metadata. The robustness of the system is then evaluated with a subset of the World Ocean Database (WOD18) with over 600,000 in-situ temperature and salinity profiles. This system is an open-source Python package allowing users to effectively use the software. Users can customize their settings. The application result from the WOD18 subset also forms a benchmark dataset, which is available to support future studies on duplicate checking, metadata error identification, and machine learning applications. This duplicate checking system will be incorporated into the International Quality-controlled Ocean Database (IQuOD) data quality control system to guarantee the uniqueness of ocean observation data in this product.

How to cite: Song, X., Tan, Z., Locarnini, R., Simoncelli, S., Cowley, R., Kizu, S., Boyer, T., Reseghetti, F., Castelao, G., Gouretski, V., and Cheng, L.: DC_OCEAN: An open-source algorithm for identification of duplicates in ocean databases, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5448, https://doi.org/10.5194/egusphere-egu25-5448, 2025.

The autonomous and remotely vehicles (ARV) plays a crucial role in deep-sea and large-scale surveying and sampling missions, which requires accurate marine spatial positioning and navigation information. Generally, the integration of ultra-short baseline (USBL) acoustic positioning system, strap-down inertial navigation system (SINS) and Doppler velocity logger (DVL) is consistently recommended for underwater geo-referencing. This inertial-acoustic fusion offers superior accuracy and reliability in determining vehicle position, speed, and attitude. However, the temporal variation of sound speed structure (SSS) emerges as a critical factor that limits the USBL positioning performance within operational areas, thereby compromising the fusion accuracy of integrated navigation systems. In this contribution, we propose a novel in-situ sound speed structure correction scheme for SINS/USBL integrated navigation. Firstly, the temporal variation of SSS based on USBL positioning functional model is analyzed, and a two-dimensional temporal SSS model is constructed. Subsequently, a novel adaptive two-stage information filter algorithm is proposed, which estimates the perturbation of the sound speed while simultaneously detecting and identifying outlier observations from both the USBL and DVL. Finally, the effectiveness of the improved method is verified through simulations and trails conducted in the South China Sea. The experimental results demonstrate that the proposed method effectively estimates the sound speed disturbance in real-time, significantly enhancing the performance of tightly integrated inertial-acoustic navigation systems.

Keywords SINS/USBL, sound speed structure, adaptive two-stage information filter, integrated navigation

How to cite: Liu, H.: An in-situ sound speed structure correction scheme for the tight integration of SINS/USBL/DVL in Deep-sea ARV navigation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7931, https://doi.org/10.5194/egusphere-egu25-7931, 2025.

EGU25-9337 | ECS | Orals | GI5.3

Clustering Soil Health Across Europe Using LUCAS Soil Dataset and Unsupervised Learning Techniques 

Ernesto Sanz, Andrés F. Almeida-Ñauñay, José M. Soriano Disla, Barbara Soriano, Isabel Bardají, and Ana M. Tarquis

Soil health is a critical factor influencing ecosystem functions, agricultural productivity, and environmental sustainability. However, the spatial variability of soil properties across Europe poses significant challenges to understanding and managing soil health at regional and continental scales. This study utilizes clustering techniques to analyze and classify soil health across Europe using the LUCAS (Land Use and Coverage Area Frame Survey) soil dataset, one of the most comprehensive databases of soil properties in Europe.

The LUCAS dataset includes key physical, chemical, and biological soil indicators such as soil organic carbon (SOC), pH, texture, and bulk density, providing a robust foundation for clustering. Data preprocessing involved standardizing soil attributes and addressing missing values through imputation. Clustering algorithms were applied to group soils with similar health profiles, capturing spatial patterns and interrelations among soil properties. The resulting clusters were mapped and analyzed to identify dominant soil health characteristics and their distribution across Europe.

Preliminary results reveal distinct clusters reflecting gradients in soil fertility, organic matter content, and degradation levels. These clusters align with known ecological and climatic gradients, validating the methodology and providing insights into the spatial variability of soil health. Furthermore, this clustering approach highlights regions requiring targeted soil management interventions, contributing to data-driven decision-making for sustainable land use and agricultural practices.

This research demonstrates the potential of unsupervised learning to leverage large-scale datasets for spatial soil health analysis, offering a scalable framework for soil health monitoring and management at regional and continental scales. Future work will incorporate temporal data to assess changes in soil health over time, further enhancing the utility of this approach in dynamic soil monitoring systems.

Keywords—soil health, soil indicators, random forest, agriculture, soil monitoring

Acknowledgements: The iCOSHELLs project is funded by the European Union. Views and opinions expressed are however those of the author(s) only and do not necessarily reflect those of the European Union or the European Research Executive Agency (REA). Neither the European Union nor the granting authority can be held responsible for them.

References: Sanz, E., Sotoca, J. J. M., Saa-Requejo, A., Díaz-Ambrona, C. H., RuizRamos, M., Rodríguez, A., & Tarquis, A. M. (2022). Clustering arid rangelands based on NDVI annual patterns and their persistence. Remote Sensing, 14(19), 4949.

Boluwade, Alaba (2019). Regionalization and partitioning of soil health indicators for Nigeria using spatially contiguous clustering for economic and social-cultural developments. ISPRS International Journal of Geo-Information 8.10: 458.

Suchithra, M. S., and Maya L. Pai (2020). Data mining based geospatial clustering for suitable recommendation system. 2020 International Conference on Inventive Computation Technologies (ICICT). IEEE.

 

How to cite: Sanz, E., Almeida-Ñauñay, A. F., Soriano Disla, J. M., Soriano, B., Bardají, I., and Tarquis, A. M.: Clustering Soil Health Across Europe Using LUCAS Soil Dataset and Unsupervised Learning Techniques, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9337, https://doi.org/10.5194/egusphere-egu25-9337, 2025.

EGU25-9403 | Posters on site | GI5.3

Facilitating Earth Observation: GFZ’s GNSS Instrument Pool 

Benjamin Männel, Markus Ramatschi, Markus Bradke, Eric am Mihr, and Jens Wickert

Global Navigation Satellite Systems (GNSS) like GPS or Galileo allow high-accurate positioning and geolocation. GNSS has been used in geosciences for more than three decades for surface deformation monitoring, including tectonics, earthquake cycle, and vertical land motion associated with postglacial rebound. The possibility of observing atmospheric conditions, especially electron content and water vapor distribution, allows multi-purpose applications. Thanks to modernizations in the GNSS constellations, including new signals, advanced and cost-efficient receiver equipment has been developed over the past few years. This allows the establishment of dense observation networks and advanced observation scenarios.

GFZ recently integrated GNSS receivers into the Geophysical Instrument Pool (GIPP) to support GNSS-based applications in various domains. This research infrastructure facility is open to all national and international academic applicants; the instruments are provided free of charge following a transparent application and evaluation procedure. This contribution presents the available GNSS equipment, potential applications, and the user pipeline from deployment to results. Results from two supported projects will be presented in more detail. The first focuses on surface deformation across the Irpinia and Pergola-Melandro fault system and the second on monitoring seasonal acceleration at the 79°N Glacier in Greenland. Both examples highlight the value of accurate, in-situ coordinate time series.

How to cite: Männel, B., Ramatschi, M., Bradke, M., am Mihr, E., and Wickert, J.: Facilitating Earth Observation: GFZ’s GNSS Instrument Pool, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9403, https://doi.org/10.5194/egusphere-egu25-9403, 2025.

EGU25-10397 | ECS | Posters on site | GI5.3

Soil Characterization Using Gamma-Ray Spectrometry: Caste study in Petzenkirchen, Austria 

Matthias Konzett, Peter Strauss, and Elmar Schmaltz

Soil physical and chemical parameters—such as texture, density, water content, total organic carbon (TOC), and total nitrogen (TN)—are typically measured at a single point and then extrapolated to represent a larger area. To accurately characterize these areas, a substantial number of samples must be collected, which can lead to high laboratory costs. Using a UAV-borne gamma-ray spectrometer at relatively low altitudes allows for collecting high-resolution spatial information on radionuclides. This information may subsequently be used to derive soil physical and chemical parameters.

In the Hydrological Open-Air Laboratory (HOAL) in Petzenkirchen, Lower Austria, a Medusa gamma-ray MS-1000 was employed to test the potential of obtaining continuous soil information on basic soil properties. The gamma-ray spectrometer was mounted on an Acecore NOA UAV and a backpack, enabling users to remotely fly or walk across the area of interest, respectively. The study focused on three land-use types: agricultural land – covered by winter wheat in an early development stage, 3-year-old grassland, and 10+ year-old grassland, each with an area of about 0.2 hectares. The soil in this area is classified as drained typical gley and a gleyic colluvisol. After surveying with the gamma-ray spectrometer from each land-use type, we randomly collected 10 soil samples and analyzed for texture, density, water content, TOC, and TN.

Previous research by Van der Veeke et al. (2021) and Taylor et al. (2023) provides some contradictory context to this experiment. Van der Veeke et al. (2021) achieved R² values greater than 0.8 for clay and sand content compared to measured soil data. In contrast, Taylor et al. (2023) obtained correlation coefficients ranging from -0.59 to 0.61 but received better values of about -0.71 or lower for soil moisture, total carbon and TN. This study aims to offer a more definitive conclusion in predicting soil physical and chemical parameters using gamma-ray spectrometry.

How to cite: Konzett, M., Strauss, P., and Schmaltz, E.: Soil Characterization Using Gamma-Ray Spectrometry: Caste study in Petzenkirchen, Austria, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10397, https://doi.org/10.5194/egusphere-egu25-10397, 2025.

EGU25-11576 | Orals | GI5.3

Measuring solar radiation from a swaying balloon platform 

R. Giles Harrison

Incoming solar radiation is a fundamental atmospheric quantity, typically measured at the surface using pyranometer devices, with thermopile or semiconductor sensors. During its passage through the atmosphere, solar radiation is absorbed and scattered. One method for removing the atmospheric effects on the measured solar irradiance is Langley extrapolation, but its effectiveness for determining the top-of-atmosphere irradiance is highly dependent on the measuring circumstances. It is preferable to make in situ atmospheric measurements using an airborne platform, such as an aircraft or balloon system. A practical difficulty, however, with small platforms is their motion, for which complex stabilization approaches may be needed. An alternative approach is to monitor the platform’s motion, using the additional information to correct for the varying orientation of the sensor. To evaluate the effectiveness of this approach, a small self-contained data logger was developed to capture solar radiation measurements across a wide dynamic range, using a photodiode as a sensor. The package included an orientation sensor to allow position fluctuations to be monitored and accounted for. The system was carried on a radiosonde flight to 30 km altitude, with both solar radiation and orientation measured throughout. Combining the data streams shows that improved solar irradiance measurements can be obtained using the orientation information, without the need for physical stabilization of the carrier platform.

How to cite: Harrison, R. G.: Measuring solar radiation from a swaying balloon platform, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11576, https://doi.org/10.5194/egusphere-egu25-11576, 2025.

EGU25-12053 | Posters on site | GI5.3

Monitoring diffuse CO2 emission: a geochemical surveillance tool for Cumbre Vieja volcano, La Palma, Canary Islands, Spain  

David Afonso Falcón, Victoria Kichmerova, Katherine Smith, Raghad Ali bin Jaddua, Gladys V. Melián, Daniela Taño Ramos, Laura Trujillo Vargas, Claudia Ramos Delgado, Ana Gironés, Eleazar Padrón, María Asensio Ramos, Pedro A. Hernández, and Nemesio M. Pérez

La Palma Island (708 km²) is located in the northwestern part of the Canarian Archipelago and represents one of its youngest volcanic structures, with an estimated geological age of around 2.0 million years. On September 19, 2021, a significant volcanic eruption occurred within the Cumbre Vieja volcanic system situated in the southern region of the island. This event, lasting 85 days and 8 hours, is recorded as the longest volcanic episode in La Palma's documented history. The eruption resulted in extensive lava flows that covered an area of approximately 1,219 hectares, causing substantial geological and social impact. Since visible volcanic gas emissions (fumaroles, hot springs, etc.) do not occur at the surface environment of Cumbre Vieja, the geochemical program for the volcanic surveillance has been focused mainly on diffuse (non-visible) degassing studies. This study presents the findings from annual diffuse carbon dioxide (CO₂) emission surveys conducted since 2001, with increased monitoring frequency between 2017 and 2024 to optimize the early warning system for future volcanic eruptions at La Palma island.

The measurement of soil CO₂ efflux was performed following the accumulation chamber method across approximately 600 sampling sites distributed throughout the volcanic system. The long-term time series data reveal distinct periods of diffuse CO₂ emissions that provide valuable insights into the system's volcanic activity: (1) A baseline period (2001-2016), when diffuse CO₂ emissions fluctuated between 320 and 1,544 t/d, establishing a reference range for background degassing levels.; (2) A pre-eruptive period (2016-2021), when a marked increase in CO₂ emissions was observed, with values rising from 788 t·d⁻¹ to a peak of 1,870 t·d⁻¹. This last period coincided with the onset of seismic swarm activity, highlighting a clear correlation between increased degassing and evolving magmatic processes beneath the surface; (3) The eruptive period (2021). During the eruption, CO₂ emissions exhibited significant temporal variations. A minimum emission rate was recorded on October 21, followed by a sharp increase that peaked at 4,435 t·d⁻¹ on December 14, aligning with the conclusion of the eruptive phase. This maximum emission rate represents the highest value observed in the entire monitoring serie; and (4) the post-eruptive period (2022-2024), when diffuse CO₂ emissions showed a decreasing trend, stabilizing around 760 t·d⁻¹, reflecting a gradual return to lower degassing levels.

These findings underscore the critical importance of continuous diffuse CO₂ monitoring as a key component of volcanic surveillance at Cumbre Vieja. Regular measurements of diffuse gas emissions provide essential early warning indicators of potential volcanic unrest, allowing for improved risk assessment and hazard mitigation strategies. The integration of geochemical monitoring with other geophysical and geological tools enhances the comprehensive understanding of the dynamic behavior of volcanic systems.

How to cite: Afonso Falcón, D., Kichmerova, V., Smith, K., Ali bin Jaddua, R., Melián, G. V., Taño Ramos, D., Trujillo Vargas, L., Ramos Delgado, C., Gironés, A., Padrón, E., Asensio Ramos, M., Hernández, P. A., and Pérez, N. M.: Monitoring diffuse CO2 emission: a geochemical surveillance tool for Cumbre Vieja volcano, La Palma, Canary Islands, Spain , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12053, https://doi.org/10.5194/egusphere-egu25-12053, 2025.

EGU25-13765 | ECS | Orals | GI5.3

Advancing Soil and Environmental Analysis with Dual-Wavelength Raman Spectroscopy and Machine Learning  

Ginger Brown, Natalia Solomatova, and Edward Grant

Advanced environmental measurements require versatile, high-throughput methodologies that can analyze complex and heterogeneous systems. Raman spectroscopy presents a promising solution as an optical measurement technique, owing to its minimal sample preparation requirements, real-time and non-destructive measurements, and its potential for field deployment. However, its adoption in environmental applications has been limited by challenges such as fluorescence interference and sample heterogeneity. Here, we describe a dual-wavelength Raman spectroscopy approach that overcomes these challenges, enabling precise and reliable measurements of soil. Central to our approach is a custom Shifted-Excitation Raman Difference Spectroscopy (SERDS) instrument, which integrates advanced optical design, signal processing, and machine-learning multivariate analysis. 

We utilize our SERDS methodology to measure soil organic carbon (SOC) in agricultural soils and tire wear particles. By leveraging custom spectral collection strategies and signal processing tools, such as common-mode rejection (CMR) along with hyperspectral data fusion techniques, we effectively mitigate fluorescence interference, particle size variations, and nonlinear optical behavior in soils for accurate SOC and tire wear quantification. Nonlinear machine-learning regression techniques, including tree-based models and a custom Partial Least Squares Regression algorithm, enhance predictive accuracy and validate the methodology. 

While the measurement of SOC and tire wear particles in soil highlight the potential of our SERDS methodology in advancing real-time and high-throughput soil measurements, its versatility extends to a broad range of environmental sensing applications, including water quality monitoring, pollutant detection, and the analysis of complex environmental systems. This research presents an in-depth examination of the design and implementation of the SERDS instrument and methodology, showcasing its potential for advancing environmental measurement and its adaptability for addressing a wide range of analytical challenges in environmental science.

How to cite: Brown, G., Solomatova, N., and Grant, E.: Advancing Soil and Environmental Analysis with Dual-Wavelength Raman Spectroscopy and Machine Learning , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13765, https://doi.org/10.5194/egusphere-egu25-13765, 2025.

EGU25-16184 | Posters on site | GI5.3

Measuring ocean turbulence under extreme storm conditions using helicopter-deployed ocean gliders 

Daniel Carlson, Lucas Merkelbach, and Jeff Carpenter

Climate change is expected to increase the frequency and intensity of extreme weather events, with dire socioeconomic impacts for coastal communities. Efforts to improve forecasts of storms are impeded by a lack of ocean mixing observations under extreme storm conditions. Observations, while risky, are necessary to develop accurate parameterizations of storm-driven ocean mixing. Extreme storms, like tropical cyclones, create conditions that exceed operational safety thresholds for crewed oceanographic research vessels, making uncrewed vehicles, like ocean gliders, a more sensible measurement platform. While uncrewed gliders remove the risk to humans, they must still be deployed at the right place and at the right time. Storm systems can develop and change quickly, requiring a fast, flexible and adaptable deployment strategy. Slow-moving research vessels, which must also seek shelter from approaching storms, are ill-suited for this task. Civil helicopter aviation companies currently serve the offshore energy segment, ferrying crews and equipment between shore-based airfields and offshore infrastructure. Here, we explore the use of helicopters for the deployment of ocean gliders in the paths of extreme storm systems. While helicopters have the speed and flexibility required for rapid, on-demand glider deployments, these activities are far from routine, requiring the development of deployment strategies that ensure the safety of the aircraft and flight crew as well as the safe deployment of the sensitive microstructure sensors required to measure ocean turbulence and mixing. We report on initial collaborations with the aviation industry and the development of procedures to deploy and retrieve ocean gliders from helicopters.

How to cite: Carlson, D., Merkelbach, L., and Carpenter, J.: Measuring ocean turbulence under extreme storm conditions using helicopter-deployed ocean gliders, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16184, https://doi.org/10.5194/egusphere-egu25-16184, 2025.

EGU25-16798 | ECS | Orals | GI5.3

A Novel Methodology for Deployment and Retrieval of Autonomous Deep Ocean Distributed Acoustic Sensing Landers and Submarine Cable Layout 

Ignacio Robles Urquijo, César González-Pola, Luis Rodriguez-Cobo, Jose J. Valdiande, Rocio Grana, and Adolfo Cobo

This study presents an innovative approach for the deployment and retrieval of autonomous deep ocean landers equipped with Distributed Acoustic Sensing (DAS) systems and associated fiber optic cables. The methodology utilizes the LanderPick system, a Remote Operated Towed Vehicle (ROTV), to facilitate precise placement and recovery of the lander and measuring cable on the seafloor. The integrated DAS system employs fiber optic technology to provide high-resolution acoustic monitoring along the cable's length, facilitating long-range detection of various underwater phenomena.

The autonomous lander design incorporates a frame structure and pressure-resistant housing designed to withstand depths of up to 6,000 meters. A key feature of the method is the lander’s hitching mesh and attached fiber optic reel mechanism, which enables controlled deployment and laying of the measured fiber. A specialized housing protects the DAS interrogator and associated electronics from the harsh deep-sea environment, ensuring long-term operational reliability.

The LanderPick deployment system, an ROTV, enables precise placement and recovery of the lander on the seafloor, while the attach reel mechanism allows to steer the cable layout as required. This approach significantly enhances the survivability and accuracy of the deployment process while allowing for continuous monitoring of the optic fiber deployment.

This novel approach addresses limitations of onshore installations utilizing submarine telecommunication cables, which often lack the location and fiber layout flexibility required for measuring specific ocean areas of interest. By enabling the deployment of autonomous platforms with customizable cable layouts, this solution significantly expands the potential applications of distributed sensing techniques in undersea environments.

Field trials have successfully demonstrated the LanderPick's capability to conduct deployment and retrieval missions with real time visual feedback. The adaptation of this controlled deployment method to the distributed sensing requirements represents an opportunity for deep-sea observation techniques, offering new opportunities for long-term monitoring of benthic ecosystems and geophysical processes. In conclusion, this innovative methodology for deploying and retrieving autonomous deep ocean DAS landers, coupled with customizable submarine cable layouts, has the potential to revolutionize underwater sensing and monitoring capabilities across a wide range of scientific and industrial applications.

How to cite: Robles Urquijo, I., González-Pola, C., Rodriguez-Cobo, L., Valdiande, J. J., Grana, R., and Cobo, A.: A Novel Methodology for Deployment and Retrieval of Autonomous Deep Ocean Distributed Acoustic Sensing Landers and Submarine Cable Layout, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16798, https://doi.org/10.5194/egusphere-egu25-16798, 2025.

EGU25-16799 | Posters on site | GI5.3

Successful Deployment of a 21km SMART Cable with Force-Feedback Seismometer and Accelerometers in the Mediterranean Sea 

Jamie Calver, Neil Watkiss, Federica Restelli, Antoaneta Kerkenyakova, and Sally Mohr

Autonomous Ocean Bottom Seismometer (OBS) deployments have often involved a degree of “drop-and-hope” due to the inherent lack of seismic data communication during installation as well as waiting extended periods before data collection. Cabled solutions provide real-time data during and immediately after deployment, sometimes with opportunity to adjust the instrument before it is left to operate remotely. However, cabled solutions are inherently financially and logistically challenging both in terms of seismic hardware and arguably more significantly, deployment hardware (ships, ROVs, cables etc.). The geographical reach of these experiments is also often limited to within a few hundred kilometres of the coast. These constraints often mean cabled OBS are beyond the scope of most scientific bodies.

Güralp Systems Limited, in collaboration with the Istituto Nazionale di Geofisica e Vulcanologia (INGV), has successfully manufactured and demonstrated a method of reducing financial and logistical constraints, extending geographical range, and crucially maintaining data quality by utilising force-feedback seismic instrumentation in cabled OBS systems. The recent successful deployment of the InSEA Wet Demo SMART (Science Monitoring And Reliable Telecommunications) cable, off the coast of Sicily, displays a world first in how science can partner with industry to achieve this.

SMART cables are primarily telecommunication cables that secondarily serve as hosts for scientific monitoring equipment. Commercial viability for these systems relies on the cable being laid as if the science element did not exist, thereby minimising additional deployment costs and reducing barriers to cooperation with cable laying companies. Güralp and INGV deployed 3 seismometer-accelerometer pairs housed inline within the cable repeater housings along the 21km cable length using standard cable-laying techniques to show proof of concept. The system also features a series of high-performance temperature and pressure sensors that can be used for larger scale oceanographic monitoring.

This pioneering installation using telecommunication cables marks a significant step towards drastically improving local knowledge of inaccessible oceanic regions as well as global azimuthal coverage for teleseismic events, all in real time.

How to cite: Calver, J., Watkiss, N., Restelli, F., Kerkenyakova, A., and Mohr, S.: Successful Deployment of a 21km SMART Cable with Force-Feedback Seismometer and Accelerometers in the Mediterranean Sea, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16799, https://doi.org/10.5194/egusphere-egu25-16799, 2025.

EGU25-16802 | Orals | GI5.3

An Integrated Real-Time MultidisciplinaryGeophysical Borehole Observatory 

Cansun Guralp and Murray McGowan

The world's first integrated geophysical borehole observatory has been installed by GaiaCode on the Kapidag Peninsula on the South coast of the Marmara Sea in Türkiye (40O29'22” N, 27O58'44” E). The downhole instrumentation consists of a low noise ultra-broadband three component feedback seismometer, a strain-meter, a dilatometer, a continuous pore-pressure sensor and a temperature probe. All these instruments and sensors were designed and built in house by GaiaCode. To complete the observatory, these sensors will be augmented by a MEMS accelerometer and a three axis 4.5 Hz geophone installed downhole as well as a weather station at the well head. The latter instruments were supplied by other vendors but integrated into the observatory by us.

 

The observatory has two boreholes which are about 4 m apart. Each hole is approximately 110 m deep with minimal vertical deviation. The first set of instruments (dilatometer, strain-meter and a set of borehole geophones) has been cemented into the bottom of the first borehole. The ultra broadband seismometer “ALPHA” with 360 seconds low frequency corner and 200 Hz upper frequency corner with 5 decades of frequency range  will be installed in a special casing in the same borehole.

 

This seismometer will also serve as a downhole tilt-meter, using its mass position outputs. Unlike triaxial (tilted Galperin) seismometer, classic orthogonal topology has the advantage over tilted Triaxial Galperin seismometers of providing precision tilt measurement without the requirement of a separate expensive tilt sensor. The broadband seismometer is equipped with a stable  single jaw hole-lock for easy retrieval. The real time pore-pressure sensor will be cemented into the second borehole.

 

The analogue measurements from these instruments will all be transmitted to their respective well head, where they will be processed by a fleet of TAU digitizers. TAU digitises can transmit 6 concurrent sample rates, ideally suited for Multidisciplinary seismic station data acquisition. Gaiacode's OMEGA software is used for recording and controlling-configuring the sensor system and the digitisers.

 

This new observatory is a major extension of the joint research initiative by the German Geoscience Research Center (GFZ) and the Turkish Disaster and Emergency Management Presidency (AFAD): the GONAF Project (Geophysical Observatory at the North Anatolian Fault). Its main objective is to measure seismic and aseismic tectonic deformation transients along the Marmara section of the North Anatolian Fault in northwestern Türkiye. This section is overdue for a major earthquake. The observatory will be jointly operated by GFZ and AFAD.

How to cite: Guralp, C. and McGowan, M.: An Integrated Real-Time MultidisciplinaryGeophysical Borehole Observatory, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16802, https://doi.org/10.5194/egusphere-egu25-16802, 2025.

EGU25-16946 | ECS | Posters on site | GI5.3

Spatio-temporal patterns in repeated spontaneous potential measurements in the crater of Teide volcano (Tenerife). 

Rubén García Hernández, Ástor Fernández-Carballo, Barbara Mandato, Sreenidhi Prabagaran, Aarón Álvarez, Luca D'Auria, David Martínez van Dorth, Víctor Ortega-Ramos, and Nemesio M. Pérez

The analysis of multiparametric geophysical and geochemical datasets presents significant challenges due to the diverse nature of measurements and their potential interactions. The development of advanced statistical and data mining techniques has enabled researchers to identify and characterise complex patterns within such datasets. This work builds upon a previous study that applied Independent Vector Analysis (IVA) to analyse multiparametric measurements collected at Teide volcano crater (Tenerife, Canary Islands) between 2020 and 2024. Our main goal is to extend the initial findings by identifying endogenous and exogenous factors influencing the observed patterns and characterising their temporal behaviour.

The dataset includes spontaneous potential, CO2 and H2S fluxes, and thermal gradient measurements taken within the crater of Teide volcano on 38 fixed points. The application of IVA, which is an extension of Independent Component Analysis (ICA), allows for a multivariate approach that leverages vectorial data instead of scalar quantities. This method has proven effective for disentangling spatio-temporal interactions and isolating independent processes that govern the observed geophysical and geochemical variations.

Based on previous preliminary results, this study incorporates new data collected during 2023 and 2024, allowing a better definition of the spatio-temporal patterns. Using the IVA, we identify and quantify evolving endogenous patterns potentially related to magmatic processes. Simultaneously, we assess the influence of exogenous factors such as seasonal temperature fluctuations and hydrological changes.

Our results highlight the robustness of IVA in separating and characterising independent processes contributing to spatio-temporal multivariate datasets, such as the specific case of the Teide volcano. The results reveal a strong correlation between spontaneous potential anomalies and localised gas emissions, validating this methodology in volcanic environments. Moreover, this extended study underscores the importance of integrating temporal dynamics into multivariate analyses to improve the understanding of volcanic systems.

This work demonstrates the potential of IVA as a powerful tool for analysing repeated geophysical and geochemical surveys. It offers significant advantages for monitoring active volcanic systems. Future applications could include adding more datasets, such as remote sensing and/or other geophysical or geochemical parameters, to understand volcanic processes comprehensively.

How to cite: García Hernández, R., Fernández-Carballo, Á., Mandato, B., Prabagaran, S., Álvarez, A., D'Auria, L., Martínez van Dorth, D., Ortega-Ramos, V., and Pérez, N. M.: Spatio-temporal patterns in repeated spontaneous potential measurements in the crater of Teide volcano (Tenerife)., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16946, https://doi.org/10.5194/egusphere-egu25-16946, 2025.

EGU25-17775 | Posters on site | GI5.3

Continuous monitoring of diffuse degassing at the summit cone of Teide volcano, Tenerife, Canary Islands 

María Asensio-Ramos, Daniel Di Nardo, Gladys V. Melián, Germán D. Padilla, Pedro A. Hernández, Eleazar Padrón, and Nemesio M. Pérez

The chemical composition of volcanic gases provides essential insights into the activity and dynamics of volcanic systems, as well as the magmatic and hydrothermal processes occurring at depth. These gases, including CO2, H2, CH4, and H2S, are key indicators of physical and chemical processes such as redox reactions and magmatic degassing. Furthermore, the relative concentrations and ratios of specific gas species offer valuable information for interpreting subsurface dynamics and detecting changes in volcanic activity.

In recent decades, researchers have made significant efforts to measure gas concentrations and fluxes in volcanic fluids. However, continuous monitoring of gas emissions and their ratios in active volcanoes remains limited. Here, we present results from a continuous monitoring station (CMS) installed in November 2017 on the southeastern flank of Teide volcano. This station monitors the ground gas atmosphere using a device that collects samples at a depth of 10 cm, measuring CO2, H2, He, H2S, CH4, and other gases to analyze their temporal evolution and interrelationships. The data collected spans from its installation to the present day, providing a comprehensive record of gas behaviour over time.

The CMS is equipped with an Agilent 490 micro-GC with two channels, capable of analyzing He, Ne, H2, O2, N2, CH4, CO2 and H2S. The system includes an embedded computer with internet connectivity (via WiFi or UMTS router), enabling full remote control of the instrument, automatic data transmission, and automated gas sampling.

High concentrations of CO2 (with a moving average exceeding 60% for most of the measurement period), H2 (above 1,200 ppm), He (above 10 ppm), and H2S (above 1,000 ppm) highlight significant temporal trends linked to variations in volcanic and hydrothermal activity. The analysis of gas ratios, such as He/CO2, H2/CO2, and H2S/CO2, shows fluctuations consistent with changes in volcanic activity. Decreases in atmospheric gases like N2 and O2 often coincide with increases in magmatic components, reinforcing the utility of gas ratios in understanding subsurface processes.

This CMS constitutes a robust system for volcanic monitoring, capable of detecting low concentrations of key gases and providing critical insights through the analysis of both gas concentrations and their ratios. Such tools are invaluable for advancing volcanic surveillance and risk assessment.

How to cite: Asensio-Ramos, M., Di Nardo, D., Melián, G. V., Padilla, G. D., Hernández, P. A., Padrón, E., and Pérez, N. M.: Continuous monitoring of diffuse degassing at the summit cone of Teide volcano, Tenerife, Canary Islands, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17775, https://doi.org/10.5194/egusphere-egu25-17775, 2025.

EGU25-17935 | ECS | Posters on site | GI5.3

Implementation of a prototype monitoring system to investigate post-fire geomorphic processes   

Niccolò Dematteis, Marco Cavalli, Rosa Maria Cavalli, Stefano Crema, Michele De Biase, Marco Donnini, Giuseppe Esposito, Stefano Luigi Gariano, Marco Piantini, Luca Pisano, and Mauro Rossi

The current abstract presents experimental analyses and monitoring to studying post-fire geomorphic processes, a potential indirect effect of wildfires. The primary goal is to identify environmental variables that could serve as indicators for triggering post-fire soil erosion and mass wasting in mountain watersheds.

Two pilot sites were chosen in southern Italy, and specifically in mountain regions severely affected by wildfires in the last years. The monitored environmental quantities include i) meteorological variables – precipitation, air temperature, wind speed and direction, lighting, barometric pressure and solar radiation – detected by modern all-in-one automatic weather station and a traditional tipping bucket rain gauge. ii) Soil moisture content and temperature measured by TDR sensors 10 cm-deep and Cosmic Ray Neutron Sensing. iii) Local seismicity measured by triaxial geophones. iv) Surface optical and thermal evolution using a combined RGB+thermal video camera.

Key research topics being tested include: 1) the application of image change detection techniques to analyze runoff, soil erosion, and landslides during post-fire rainstorms using visual and thermal imagery; 2) the use of a triaxial seismic sensor to capture ground vibrations and characterize sediment-laden turbulent flows; 3) spatial estimation of soil moisture conditions preceding post-fire geomorphic events; and 4) lightning detection to anticipate the approach of convective cells at the monitored sites. Alongside these positive aspects, the research team is addressing several challenges, such as managing remote control and communication, storing data locally, and ensuring reliable power supply.

Preliminary results obtained with the RGB+thermal images and seismic data, which have been acquired during a series of rainfall events that triggered soil erosion, small rock falls and hyperconcentrated flows suggest that the involved instrumentations can represent a valuable tool in monitoring mass wasting processes linked to intense precipitations after wildfires. Future testing and implementations should contribute to develop an innovative monitoring system to assist public authorities in managing post-fire risks.

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

How to cite: Dematteis, N., Cavalli, M., Cavalli, R. M., Crema, S., De Biase, M., Donnini, M., Esposito, G., Gariano, S. L., Piantini, M., Pisano, L., and Rossi, M.: Implementation of a prototype monitoring system to investigate post-fire geomorphic processes  , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17935, https://doi.org/10.5194/egusphere-egu25-17935, 2025.

EGU25-18318 | Posters on site | GI5.3

Revised 3D crustal structure of Southern Italy: an integrated approach combining geophysical and petrophysical constraints 

Raffaele Castaldo, Maddalena Perrini, Filippo Accomando, Grazia De Landro, Gianluca Gola, Pietro Tizzani, Michele Carafa, Maurizio Fedi, Aldo Zollo, Vanja Kastelic, Cinzia Di Lorenzo, Deborah Di Naccio, and Matteo Taroni

The Southern Italy, a tectonically active region of significant geodynamic importance, is also a critical area for seismic hazard assessment and sustainable resource management. Characterized by lithospheric convergence, crustal delamination, active fault systems and a complex tectonic style made up of the eastward thrusting of different, once adjacent, geographic paleo-domains, the area faces considerable seismic risks. These features make the Southern Apennines, and thus the Southern Italy, an ideal yet complex laboratory for constructing an integrated 3D geometrical model to address structural complexities and support hazard mitigation efforts, where the significance of the results justifies the challenges inherent in the integration process.

This study integrates geological and geophysical data to develop an integrated 3D crustal model for the Southern Apennines area, with a spatial resolution of 5x5x1 km3, along East, North and depth, respectively. Our analysis synthesizes stratigraphic, geophysical, and structural data into a unified framework for regional geological interpretation. Key datasets include stratigraphic well logs (ViDEPI project consultable at the page: https://www.videpi.com/videpi/pozzi/pozzi.asp), lithological maps, seismic tomographic models, gravity and magnetic models, and thermal and petrophysical constraints. These datasets underwent rigorous filtering, analysis and gridding to ensure consistency across spatial scales. The methodology incorporates thermal varying gradients, P-wave velocity variations, and depth-dependent corrections, enabling the identification of major intra-crustal discontinuities and lithological transitions.

Model construction involved delineating the main lithological units, including sedimentary covers, carbonate platforms, and crystalline basement domains, extending down to the Moho depth. Validation was performed by comparing model outputs with independent borehole data and geophysical data interpretation, achieving high accuracy and resolution. By synthesizing diverse datasets into a cohesive framework, this study addresses gaps in lithologic unit characterization throughout the study area and subsurface property predictions.

The Integrated 3D geological model is a versatile tool for addressing both scientific and social challenges. It supports thermo-rheological modelling, enabling detailed analyses of brittle-ductile transitions and their implications for seismic hazards. These results represent some of the goals of the PRIN2022 PNRR entitled “Relation between 3D Thermo-Rheological Model and Seismic Hazard for Risk Mitigation in the Urban Areas of Southern Italy – TRHAM”. The model also holds significant promise for practical applications, such as green energy initiatives, particularly geothermal resource exploration, by linking geodynamic processes to sustainable development in Southern Italy.

How to cite: Castaldo, R., Perrini, M., Accomando, F., De Landro, G., Gola, G., Tizzani, P., Carafa, M., Fedi, M., Zollo, A., Kastelic, V., Di Lorenzo, C., Di Naccio, D., and Taroni, M.: Revised 3D crustal structure of Southern Italy: an integrated approach combining geophysical and petrophysical constraints, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18318, https://doi.org/10.5194/egusphere-egu25-18318, 2025.

In Chiba Prefecture, Japan, land subsidence in sub-urban regions has become an environmental and social issue which insists frequent monitoring for impact assessment. The inception of land subsidence in this region is attributed to natural factors, such as seismic activity and soil layer consolidation, as well as man-made factors, such as ground water and natural gas extraction. However, accurate estimation of the widely and distinctly distributed multiscale subsidence areas becomes very challenging, time-consuming, and labour-intensive by conventional level survey measurements. In this study, we applied and validated a ground subsidence monitoring method for Chiba Prefecture, Japan, using L-band ALOS-2 space-borne Synthetic Aperture Radar (SAR) satellite data. We used Single Look Complex SAR data in StripMap mode with a 3 m resolution, a swath width of 70 km, and repeat-pass acquisition geometry. Continuously acquired ALOS-2 SAR data in both ascending and descending orbital directions, totally 78 scenes were used from 2016 to 2023. The small baseline subset method was used to stack the interferograms and reduce the phase distortions, and convert them into the corresponding vertical displacement for subsidence measurements. The estimated time-series subsidence results were further assessed for areas with high coherency (> 0.6). The estimated annual subsidence rate from SAR-based measurements confirms the existence of certain land areas where the annual displacement exceeds -15 mm per year and their spatial extent. We used the least-squares method for spatial data with four adjustment parameters to improve the overall accuracy of SAR-based subsidence measurements by integrating them with the sparsely distributed 309 level survey locations. The results were categorized into six classes based on the annual subsidence rates, and the root-mean-square error (RMSE) was compared before and after the improvement of subsidence measurements using the proposed method. The results indicate that the RMSE for each subsidence class is below 5 mm, confirming consistency with national accuracy standards for subsidence monitoring.

How to cite: Karunathilake, A.: Monitoring and modelling of progressive land subsidence using multi-temporal space-borne remote sensing measurements , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18444, https://doi.org/10.5194/egusphere-egu25-18444, 2025.

EGU25-19102 | ECS | Orals | GI5.3 | Highlight

Advanced Boundary Analysis techniques as a tool to decipher volcano-tectonic setting of the Campi Flegrei caldera 

Maddalena Perrini, Andrea Barone, Pietro Tizzani, and Raffaele Castaldo

Faults are essential structures in the Earth's crust, playing a key role in regulating subsurface fluid flow and driving crustal deformation. In volcanic regions, they facilitate the migration of magma and fluids, significantly influencing volcanic processes and associated deformation patterns. Understanding the interplay between deformation patterns, subsurface heterogeneities, and fault structures is critical for accurately interpreting local volcanic dynamics, situating them within broader geodynamic frameworks, and assessing potential hazards. Boundary analysis techniques, traditionally applied to potential field data, are effective tools for investigating subsurface heterogeneities. Key methods include the Total Horizontal Derivative (THD), Tilt Angle of Horizontal Gradient (TAHG), and Normalized Total Gradient (NTG). Among these, THD has proven particularly valuable for detecting deformation sources in volcanic regions. Specifically, at Campi Flegrei caldera (CFc), THD has been applied to gravity and magnetic data as well as InSAR-derived deformation measurements, effectively aiding in the precise identification of the extent of the local volcanic source of deformation. This study integrates boundary analysis techniques (THD, TAHG, and NTG) with seismic tomography results and InSAR deformation data to conduct a comprehensive structural analysis of CFc and surrounding land and marine areas. Using datasets from mid-2021 to mid-2022, we delineate surface and subsurface structures, correlate them with major tectonic trends, and analyze their relation to local seismicity. Seismic tomography data from Giacomuzzi et al. (2024) provide 3D insights into seismic velocity distributions, highlighting crustal heterogeneities and structural weaknesses. To enhance interpretation, Total Horizontal Derivative (THD) emphasizes shallow features like faults and lithological contacts, while Tilt Angle of Horizontal Gradient (TAHG) and Normalized Total Gradient (NTG) analyze vertical deformation from InSAR data, improving sensitivity to deeper structures and minor heterogeneities. These techniques balance resolution and minimize noise, making them particularly suited for analyzing high-resolution deformation fields. To validate these techniques, we also conducted a testing phase using synthetic simulations. Our results reveal a regionally coherent yet intricate deformation pattern, consistent with the trends outlined in existing volcano-tectonic maps. This study enhances understanding of the Campi Flegrei caldera (CFc) and highlights the broader applicability of advanced boundary analysis techniques for volcano-tectonic investigations. By integrating seismic and deformation datasets with sophisticated analytical approaches, it offers valuable insights into the spatial and functional relationships between crustal heterogeneities and deformation dynamics, establishing a foundation for future research in active, densely populated regions. 

How to cite: Perrini, M., Barone, A., Tizzani, P., and Castaldo, R.: Advanced Boundary Analysis techniques as a tool to decipher volcano-tectonic setting of the Campi Flegrei caldera, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19102, https://doi.org/10.5194/egusphere-egu25-19102, 2025.

EGU25-19641 | ECS | Posters on site | GI5.3

Exploring the capabilities of geophysical technologies of the Itineris infrastructures for multiscale investigations of the soil subsoil system. 

Andrea Barone, Francesco Mercogliano, Filippo Accomando, Giuseppe Esposito, Andrea Vitale, Raffaele Castaldo, Gianluca Gennarelli, Vincenzo De Novellis, Susi Pepe, Giuseppe Solaro, Maurizio Buonanno, Antonello Bonfante, Pietro Tizzani, and Ilaria Catapano

We here deal with technologies employing geophysical measurements to detect the soil-subsoil physical parameters distribution. In particular, we show the results of the testing of Unmanned Aerial System (UAS)- and ground-based instrumentations, such as: the magnetometer/gradiometer MagNimbus for the total magnetic field measurements (UAV-based); the Ground Penetrating Radar (GPR) Zond Aero LF (UAV-based); the multi-sensor magnetometer G-864 (ground-based); the electromagnetometer CMD Explorer 6L for the soil-subsoil electromagnetic conductivity evaluation (ground-based). The UAV-based acquisitions are performed using a DJI Matrice 300 RTK drone.

We propose the case-study of the karst plane of the Altopiano di Verteglia (AV, Southern Italy), where UAS-based measurements were performed for water pipes detection. Then, we show the tests using the G-864 system for the vertical gradient measurement of the total magnetic field at Agnano plain (Campi Flegrei caldera, Southern Italy). We also propose the application of the Frequency-Domain Electromagnetic (FDEM) method for water leakage purposes.

We finally discuss the achieved goals and the next technological challenges aimed at refining the survey protocols and strategies in the framework of the multi-scale integration for the soil-subsoil system monitoring.

This work is financed by the project ITINERIS "Italian Integrated Environmental Research Infrastructure Systems" (IR0000032), that is the Italian hub of research infrastructures in the environmental scientific domain, whose creation is supported by the national recovery and resilience plan (PNRR).

How to cite: Barone, A., Mercogliano, F., Accomando, F., Esposito, G., Vitale, A., Castaldo, R., Gennarelli, G., De Novellis, V., Pepe, S., Solaro, G., Buonanno, M., Bonfante, A., Tizzani, P., and Catapano, I.: Exploring the capabilities of geophysical technologies of the Itineris infrastructures for multiscale investigations of the soil subsoil system., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19641, https://doi.org/10.5194/egusphere-egu25-19641, 2025.

EGU25-19682 | ECS | Posters on site | GI5.3

Comprehensive modelling of the Yellowstone caldera: insights into thermal evolution, magmatic behavior, and lithospheric strength 

Maddalena Perrini, Gianluca Gola, Pietro Tizzani, Maurizio Fedi, Mouna Brahmi, and Raffaele Castaldo

The Yellowstone Volcanic Complex (YVC) in Yellowstone National Park (Wyoming, USA) attracts significant geological interest as one of the largest active continental silicic volcanic fields in the world. Despite extensive research on its high heat flow and abundant geothermal features, a detailed quantitative analysis of the brittle-ductile transition remains absent. This study aims to deepen the understanding of the subsurface geological and geophysical properties of the Yellowstone area, with a particular focus on developing an optimized lithospheric thermal profile, essential for reliable rheological and lithospheric strength analyses. Initially, the Curie isothermal surface depth was extensively mapped using high-resolution aeromagnetic data and innovative spectral analysis techniques. This mapping revealed a shallow Curie isothermal surface, ranging from 2 km to 4 km beneath the YVC. The retrieved iso-Curie depth was subsequently used as a key constraint to validate a 3D stationary Finite Element (FE) thermal model. Specifically, this isothermal surface served as experimental data for optimizing the thermal state of the crust through the Optimization Module in COMSOL Multiphysics® 6.2. The 3D model of the Yellowstone lithosphere covers approximately 40 km², with a lithospheric thickness of about 35.000  km. The domain is subdivided into three litho-thermal units: the upper crust, the lower crust, and the magmatic body. The geometry of the magmatic heat source was derived from tomographic data and incorporated into COMSOL Multiphysics® to create a consistent subsurface image of the magmatic heat source. The thermal state of the crust was simulated using the Heat Transfer in Solids Module under a purely conductive regime. To further validate the thermal model, the DBSCAN clustering algorithm was applied to analyze seismic data. A comprehensive rheological model was also developed to delineate the brittle-ductile transition within the lithospheric volume. The results revealed a brittle region well-aligned with the earthquake distribution and a complex, layered ductile zone structure, reflecting the stratified nature of the local lithospheric architecture. This study contributes to a deeper understanding of the YVC’s subsurface dynamics, offering insights into its complex geodynamic processes and providing methodologies applicable to similar studies in other volcanic and geothermally active regions with large calderas.

How to cite: Perrini, M., Gola, G., Tizzani, P., Fedi, M., Brahmi, M., and Castaldo, R.: Comprehensive modelling of the Yellowstone caldera: insights into thermal evolution, magmatic behavior, and lithospheric strength, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19682, https://doi.org/10.5194/egusphere-egu25-19682, 2025.

EGU25-3687 | ECS | Posters on site | GI5.4

Correction of Echo Spacing and Advanced Permeability Modeling for Key NMR Parameters in Overpressure and Low-Permeability Reservoirs of the YGH Basin 

He Yang, Xinmin Ge, Yajing Xu, Di Tang, Bohan Wu, and Yixiong Wu

Low-field nuclear magnetic resonance (NMR) acts as an indispensable borehole logging method for the pore size characterization and formation evaluation, including the estimation of the reservoir parameters and fluid discrimination.

The YGH basin , located in the northern South China Sea, is characterized by rapid subsidence rate, high geothermal gradient, and high formation pressure coefficient. The overpressure and low-permeability reservoirs of the YGH Basin is featured with Fine-grained lithology, elevated shale content, minute pore sizes, and complex pore structures . The NMR responses are significantly affected by measurement parameters such as echo spacing. Notable discrepancies exist between the core NMR T2 spectrum and the NMR logging T2 spectrum. Key parameters derived from NMR logging, such as the T2 geometric mean and fractal dimension, fail to accurately represent the true characteristics of the rock, thereby posing substantial challenges for precise permeability evaluation.

For better estimating the reservoir permeability using the low field NMR logging data, we conducted comprehensive petrophysical measurements such as NMR, CT scanning, grain size analysis, and mercury injection capillary pressure(MICP), specifically tailored to the characteristics of overpressure and low-permeability reservoirs. Pore structure parameters were extracted from these petrophysical experiments, and the self-organizing map (SOM) unsupervised clustering method was employed to classify the pore structures of overpressure and low-permeability reservoirs. Based on the principle of phase control, multiple sets of echo spacing core NMR experiments were conducted on representative samples of different pore structure types. Systematic analysis of echo spacing 's impact on T2 spectra lead to the development of an empirical model relating T2 geometric mean, fractal dimension, and echo spacing, with a focus on the shortest echo spacing of 0.2 ms. This model provides essential data support for correcting T2 geometric mean and fractal dimension derived from NMR logging. Building on this research, the traditional Timur formula was refined by fractal dimension, significantly enhancing the accuracy of permeability calculations for overpressure and low-permeability reservoirs.

The research findings indicate that there exists a negative correlation between the T2 geometric mean value and fractal dimension, with respect to the echo interval. As the pore diameter of the rock diminishes, the porosity intensifies, accompanied by an augmentation in clay content, leading to a greater influence of echo spacing on the geometric mean of T2 and fractal dimension. By employing an enhanced permeability model, the derived permeability values demonstrate a high degree of consistency with measured data, achieving an average relative error of approximately 15%. This level of accuracy fulfills the criteria for assessing low-permeability reservoirs.

How to cite: Yang, H., Ge, X., Xu, Y., Tang, D., Wu, B., and Wu, Y.: Correction of Echo Spacing and Advanced Permeability Modeling for Key NMR Parameters in Overpressure and Low-Permeability Reservoirs of the YGH Basin, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3687, https://doi.org/10.5194/egusphere-egu25-3687, 2025.

EGU25-3893 | Posters on site | GI5.4 | Highlight

Ultra-short TE NMR One-dimensional Spatially Resolved T2 Mapping Method for Porous Media 

Xinmin Ge, Fei Wu, and Junfeng Zhao

Short T2 relaxation components are typical characteristics of porous media such as soil and rock. The ultra-short TE NMR method based on the CPMG sequence has created conditions for the overall measurement of such samples. In the evaluation of sample heterogeneity and the porous flow, in addition to the overall T2 spectrum, the 1D or multi-dimensional T2 mapping is more needed. Traditional MRI technology based on pulsed gradient field is limited by the gradient spatial encoding time and gradient eddy currents, resulting in relatively long TE, with the shortest TE being about 1.5ms, which is significantly different from the ultra-short TE required for the porous media. 1D spatially resolved T2 mapping based on constant gradient fields is a passive effect brought by the gradient magnetic field of NMR logging tools. The gradient value is not adjustable, making it difficult to regulate the layer thickness.

It is feasible to use traditional MRI gradient system combined with cooling modules to achieve 1D spatially resolved T2 mapping under constant gradient field conditions. The challenge lies in the contradiction between the Larmor frequency range in the sample selection layer direction and the -3dB bandwidth of the radio frequency coil. To address this issue, we used high Q and narrowband radio frequency coils to ensure the SNR. During 1D spatial layer selection excitation, the resonance point is tuned to match different excitation positions of the sample, or the sample position is moved to the fixed excitation frequency. Therefore, there are two technical branches, one is the radio frequency coil tuning method and the other is the sample movement method.

Since porous media have internal gradient fields, excessively high magnetic field strength will introduce internal diffusion relaxation effects. Therefore, this abstract focuses on the non-correction method which is suitable for porous media. It combines actual cases to analyze the technical features and comparison of the two branches of the non-correction method. The advantages of the tuning method are that the sample position is fixed, which is suitable for measurement conditions with peripheral accessories on the sample. The disadvantages are that the sample test length is limited, and the radio frequency hardware is complex. The advantages of the sample movement method are that the test sample length is not limited, and the radio frequency hardware is simple. The disadvantage is that sample movement is not suitable for measurement conditions with peripheral accessories. In applications, the appropriate method can be chosen according to actual needs.

How to cite: Ge, X., Wu, F., and Zhao, J.: Ultra-short TE NMR One-dimensional Spatially Resolved T2 Mapping Method for Porous Media, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3893, https://doi.org/10.5194/egusphere-egu25-3893, 2025.

EGU25-5438 | Posters on site | GI5.4

A New Protocol for Borehole NMR Simulation 

xinyu Zhang, Lizhi Xiao, Sihui Luo, and Guangzhi Liao

Nuclear magnetic resonance (NMR) logging for formation evaluation can be challenged by heterogeneity and mud filtrate invasion, leading to increased modeling errors in complex formations. Understanding the response characteristics of NMR tools at formation interfaces and their influencing factors is critical for accurate evaluation. The response of NMR logging under varying formations and instruments parameters remains unclear. This study calculates the NMR porosity decay using the Bloch equations and incorporating the spatial sensitivity distribution of the instruments.

First, the formation and borehole models were established, considering factors such as formation thickness, different formation types, mud properties, and invasion depth. The NMR measurement model was established, consisting of a permanent magnet generating a static gradient magnetic field(B0) and an RF antenna generating a radio frequency magnetic field(B1). The instrument simulated NMR responses at depths of 50 mm, 60 mm, and 70 mm. The magnetization vector decay was estimated using a recursive method based on Bloch equations. Considering the presence of non-uniform static magnetic fields or applied gradient fields, the magnetization process around the effective magnetic field. An instrument signal sensitivity calculation formula was introduced to compute the sensitivity map of the NMR signal distribution in the borehole. The total response during measurement was the combined signal contribution from different formations within the sensitive area at the time of acquisition.

This study simulated the NMR logging response under varying formation conditions, including different layer thicknesses and rock properties, while also analyzing the effects of instrument factors such as motion speed and signal-to-noise ratio (SNR). Model validation shows that the root mean square error (RMSE) of the simulation results remains below 1%. The NMR logging response is influenced by formation thickness, well deviation angle, tool motion speed, and SNR. Excessive motion speed causes incomplete polarization and echo acquisition, leading to T2 spectrum shifts proportional to antenna length. Furthermore, logging speed has a significant impact on the resolution of NMR logging; higher speeds result in reduced signal resolution. Lower SNR further degrades signal clarity, limiting the ability to distinguish pore size components during inversion and causing multiple peaks in the T2 spectrum. To optimize NMR logging, selecting appropriate logging speeds and enhancing SNR is critical for accurate lithology and porosity characterization. This research contributes to improving NMR tool performance and pre-logging planning.

How to cite: Zhang, X., Xiao, L., Luo, S., and Liao, G.: A New Protocol for Borehole NMR Simulation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5438, https://doi.org/10.5194/egusphere-egu25-5438, 2025.

EGU25-6662 | ECS | Posters on site | GI5.4

Insights into fluid types in unconventional resources reservoirs 

Xiaojiao Pang and Guiwen Wang

Lacustrine shale oil resources are crucial for maintaining energy supply. The types and contents of fluids are key factors in estimating the resource potential and oil recovery of organic-rich shales. Accurately identifying the fluid types in shale oil reservoir successions, which are characterized by significant lithological heterogeneity, is a significant challenge. Although numerous methods for determining porosity and fluid saturation have been proposed in previous studies, many are only applicable in limited situations and have limited accuracy. In this research, an advanced logging technique, Combinable Magnetic Resonance logging (CMR-NG), is employed to evaluate fluid types. Two-dimensional Nuclear Magnetic Resonance (2D-NMR) experiments were conducted on reservoir rocks under different conditions (as received, after drying at 105℃, and after kerosene imbibition) to define the fluid types and classification criteria. In addition, the contents (proportions) of various types of fluids were estimated. Subsequently, the contributions of organic matter and mineral compositions were investigated using corresponding Rock-Eval pyrolysis parameters and various mineral contents obtained from X-ray Diffraction. Then, the contents of different fluid types were calculated using CMR-NG (Combinable Magnetic Resonance logging, also known as 2D NMR logging). Based on the fluid classification criteria under experimental conditions and production data, the most favorable model and optimal solution for logging evaluation were selected. Finally, the fluid saturations were calculated for a single well. The results indicate that six fluid types (kerogen-bitumen-Group OH, irreducible oil, movable oil, clay-bound water, irreducible water, and movable water) can be recognized through the applied 2D-NMR test. The kerogen-bitumen-Group OH is mainly affected by pyrolysis hydrocarbon (S2), and irreducible oil is influenced by soluble hydrocarbon (S1). However, due to the effects of underground environmental conditions on the instruments, kerogen-bitumen-Group OH and clay-bound water cannot be detected by CMR-NG. The Q8 and Q9 layers of the Qing 2 Member of the Cretaceous Qingshankou Formation, Gulong Sag, Songliao Basin, China are identified as the most favorable layers for shale oil. This study provides insights into the factors controlling fluid types and contents, offering guidance for the exploration and development of unconventional resources, such as geothermal and CCUS (carbon capture, utilization, and storage) reservoirs.

How to cite: Pang, X. and Wang, G.: Insights into fluid types in unconventional resources reservoirs, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6662, https://doi.org/10.5194/egusphere-egu25-6662, 2025.

EGU25-7679 | ECS | Posters on site | GI5.4

Method for determining the logging speed of Improved magnetic resonance logging tool 

zhu wanli, liao guangzhi, chen wenhui, hou xueli, cao xianjun, huo dandan, and bai tao

Since the successful development of the improved magnetic resonance logging tool(iMRT), it has been well applied in complex well conditions of salinity mud and unconventional oil and gas exploration. However, the logging speed has always been the subject of discussion and research. The operation engineer expects high logging speed to improve logging efficiency, while the interpretation engineer expects lower logging speed to improve formation resolution and data quality. This article analyzes the influence of probe structure of iMRT, logging time of different observation modes, and the quality of nuclear magnetic echo signal under different mud resistivity conditions on logging speed, and establishes a calculation method. It is suitable for different geological conditions, meets the requirements of stratigraphic layering ability and high-quality data quality.

How to cite: wanli, Z., guangzhi, L., wenhui, C., xueli, H., xianjun, C., dandan, H., and tao, B.: Method for determining the logging speed of Improved magnetic resonance logging tool, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7679, https://doi.org/10.5194/egusphere-egu25-7679, 2025.

EGU25-7711 | Posters on site | GI5.4

Determination of petrophysical property cutoffs of tight lacustrine carbonate reservoir, Qaidam Basin, China 

shiming zhang, shuxin pan, guodong wang, xiaojun zhang, and juerong fu

The study area is located at the northwest end of Qaidam Basin. The exploration target horizon of the study area is the Paleogene Lower Ganchaigou Formation, which is a set of shore-shallow to semi-deep lacustrine sediments. The rock composition is characterized by the mixed deposition of argillaceous, carbonate and clastic particles.
The main reservoir types are micro- and nano-scale dolomite intercrystalline pores. a large number of intercrystalline pores were formed during the process of penecontemporaneous dolomization. Samples were taken from the drilling cores at a sampling depth of 3100m-4050m. The purpose of this method is to distinguish the movable fluid from the bound fluid by multiple centrifugation and NMR(nuclear magnetic resonance) tests, and to determine the lower limit of the pore throat radius of the movable fluid distribution according to the relation between the fluid and the pore throat, and to determine the lower limit of the physical property through the relation between the physical property and the pore throat radius.
The pore throat distribution range of the samples with carbonate intercrystalline pore in the lower Ganchaigou Formation of Yingxi area in the process of mercury injection was 11 nm to 220 nm, and the pore throat distribution range in the process of mercury ejection was 40 nm to 1500 nm.

Through saturated fluid state NMR test, it is believed that the pore throat radius of intercrystalline pore developed samples is 0-160nm, and the fluid is planar distribution, and the movable fluid accounts for 13.7%. The lower limit of pore throat containing movable fluids radius were determined to be 47nm through the separation point of accumulated curve of saturation state and centrifugal state, and it was analyzed that the lower limit of pore throat containing movable fluids were mainly affected by the median radius.The lower limit of porosity was calculated by substituting the lower limit of pore throat of movable fluid distribution into the fitting formula of the median radius of pore throat and gas porosity. There is a good correlation between permeability and test pressure. The curve of permeability and test pressure shows that when the gas permeability is less than 0.02mD, the permeability decreases rapidly with the increase of pressure, indicating that the gas flow characteristics of samples with permeability below 0.02mD and samples above 0.02mD are quite different.

How to cite: zhang, S., pan, S., wang, G., zhang, X., and fu, J.: Determination of petrophysical property cutoffs of tight lacustrine carbonate reservoir, Qaidam Basin, China, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7711, https://doi.org/10.5194/egusphere-egu25-7711, 2025.

EGU25-8799 | Posters on site | GI5.4

Application of nuclear magnetic resonance logging in Shengli shale oil reservoir 

Zhongxin Li, Chengyan Lin, and Peng Liu

The mineral composition of shale oil reservoirs in Jiyang Depression of Bohai Bay Basin, East China, is complex, the storage space is fine and tiny, and conventional logging  methods have poor applicability. Therefore, nuclear magnetic resonance logging, which can directly obtain pore information, has been widely applied in the Shengli Jiyang shale oil reservoirs. By systematically analyzing the one-dimensional and two-dimensional nuclear magnetic resonance logging data of shale oil wells in Shengli Oilfield, combined with asymmetric Gaussian function fitting technology and clustering analysis methods, the corresponding T2 cut-off values and T1/T2 value range limits for different fluid types were respectively determined. The results indicate that the pore fluid classification results of two-dimensional nuclear magnetic resonance logging are more detailed, and the movable fluid is located in the upper right corner of the spectrum, corresponding to T1/T2 values of 3 to 20. Using this model to calculate effective porosity and movable oil porosity. By comparing the tracer results, it indicates that the effective porosity of the high-yield well sections of the actual production wells was 6% to 13%, and the movable oil porosity was 2% to 6%. In other well sections, the effective porosity was less than 6%, and the movable oil porosity was less than 2%. Based on this as the main basis, the evaluation criteria for sweet spots in Shengli shale oil were established, and the shale sweet spot level was divided.

How to cite: Li, Z., Lin, C., and Liu, P.: Application of nuclear magnetic resonance logging in Shengli shale oil reservoir, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8799, https://doi.org/10.5194/egusphere-egu25-8799, 2025.

EGU25-9846 | Posters on site | GI5.4

Characterization of pore structure in tight sandstone reservoirs based on NMR 

Bing Xie, Qingsong Tang, Xun Zhu, Yuexiang Wang, and Bing Han

Tight sandstone reservoirs are characterized by low porosity, low permeability and complex pore structure, and there are difficulties in the evaluating tight sandstone reservoirs. Nuclear magnetic resonance (NMR) T2 spectra can characterize the pore structure and the fluid state of the porous medium, so we combined the NMR experiments with the gas-driven water to study the influence of different gas saturation and saturation states on the T2 spectra of the tight sandstone reservoirs. It is found that the movable peaks of T2 spectra become wider in the gas-bearing state of the pores compared with the water-bearing state, and the movable peaks decrease with the increase of gas saturation, and the porosity tends to become smaller, which is due to the lower hydrogen index of the gas. Therefore, the T2 spectrum correction model of gas-bearing sandstone reservoirs is established by combining the Gaussian distribution function, and the T2 spectrum morphology and porosity components are corrected to the original state. The T2 spectra of the NMR logging data were multi-peaked and dominated by the long relaxation component, while the gas-corrected T2 spectra were mainly two-peaked and dominated by the short relaxation component. The bound water saturation obtained from the corrected T2 spectra was basically the same with the results of the core measurements. This study combines the NMR experiments to clarify the NMR response mechanism of gas-bearing sandstone reservoirs, and establishes a Gaussian distribution model for gas-corrected T2 spectra to realize the accurate characterization of pore structure.

How to cite: Xie, B., Tang, Q., Zhu, X., Wang, Y., and Han, B.: Characterization of pore structure in tight sandstone reservoirs based on NMR, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9846, https://doi.org/10.5194/egusphere-egu25-9846, 2025.

EGU25-14149 | Posters on site | GI5.4 | Highlight

Application of low-field nuclear magnetic resonance technology in multinuclide measurements and equipment development 

liu huaxue, zhou jiapeng, liu huabing, and guo baxin

Nuclear Magnetic Resonance (NMR) technology plays a key role in many fields such as medical imaging, chemical analysis and the petroleum industry. In chemical analysis and industrial testing, the ability to measure multiple nuclides quickly and accurately is essential for productivity and quality control. Especially in key areas such as petrochemicals, materials science and environmental monitoring, there is a growing demand for equipment that can measure multiple nuclides simultaneously. However, conventional high-field NMR devices are bulky and costly, limiting their widespread use in specific application scenarios. To address these challenges, a low-field NMR-based multinuclide measurement instrument has been successfully developed in this study, which is capable of accurately measuring four nuclides, namely hydrogen (H), sodium (Na), lithium (Li), and fluorine (F), in low-field environments, and is highly integrated and suitable for a wide range of practical applications such as laboratories, on-site inspections, and industrial production lines, and supports automated data acquisition, analysis, and remote monitoring. It supports automated data acquisition, analysis and remote monitoring.

In the field of petroleum energy and civil construction materials, low-field NMR technology equipment can quickly and accurately measure and characterise the hydrogen signal, which is widely used in the structural analysis and water content determination of porous media materials, especially in pore permeability saturation testing, which supports the optimisation of the performance of petroleum extraction and civil construction materials by detecting the pore structure and permeability of the materials [1][2]. In the field of oil drilling fluids, accurate measurement of sodium (Na) ion concentration is essential to ensure drilling fluid performance. This method utilises low-field NMR technology for the non-destructive detection of Na ions in drilling fluids to safeguard the stability and efficiency of drilling fluids. In addition, during the optimisation of cement formulations, the device is able to accurately determine the change in concentration of Na ions in seawater-configured cementitious materials, thereby improving the strength and durability of the cement [3][4][5][6]. For lithium (Li), a key component in battery materials, the device is able to effectively detect lithium ion signals under low-field conditions, supporting battery R&D and materials science research to ensure continued improvement in battery performance and lifetime [7]. Fluoride (F) content is also important in the toothpaste, pharmaceutical and materials industries, and the device can quickly determine fluoride content to help optimise product formulations and ensure product quality and safety.

The electronic spectrometer system uses multiple independent RF transmitter channels, each capable of transmitting RF pulse signals with different frequencies, amplitudes or phases to suit different sample characteristics and measurement needs. The system integrates MRF (Magnetic Resonance Fingerprinting) technology and intelligent multi-classification algorithms into the host computer, which automatically captures the sample's magnetic resonance signal patterns, such as T1 and T2 relaxation times, and applies them to different field strengths and pulse sequences. With the multi-classification algorithm, the system is able to recognise and differentiate between different signal patterns, each representing a group of samples with similar properties. 

How to cite: huaxue, L., jiapeng, Z., huabing, L., and baxin, G.: Application of low-field nuclear magnetic resonance technology in multinuclide measurements and equipment development, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14149, https://doi.org/10.5194/egusphere-egu25-14149, 2025.

EGU25-14615 | Posters on site | GI5.4

A new gravity satellite constellation plan for enhancement in mid-low latitude regions 

Guangyu Jian and Min Zhong

The launch of the GRACE (Gravity Recovery and Climate Experiment) polar-orbiting gravity satellite in 2002 opened a new perspective on the mass distribution and redistribution in the Earth system, together with its successor launched in 2018, providing valuable gravity data for more than two decades. Taking its value, two established GRACE-like missions are expected to be launched and operated before 2030. Nonetheless, the high cost and insufficient spatial resolution for a GRACE-like mission continue to limit current geophysical applications, requiring an investigation into gravity satellite constellation optimization. To do so, we propose a novel gravity star network covering mid-low latitudes and put a comparison in a closed-loop simulation with the Bender constellation, showing that the new low-cost constellation may have the potential to improve the accuracy and spatiotemporal resolution of gravity field observation, opening up a new way for satellite gravity observation.

How to cite: Jian, G. and Zhong, M.: A new gravity satellite constellation plan for enhancement in mid-low latitude regions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14615, https://doi.org/10.5194/egusphere-egu25-14615, 2025.

A new method for permeability estimation in tight sandstone formations based on the BSS algorithm and NMR data is proposed. BSS algorithm is introduced into the data processing of laboratory and downhole NMR data, and relaxation components with different NMR responses and pore size distributions can be obtained. The influence of pore structure on the percolation capacity is also discussed. The new method achieves great results in tight sandstone formations.

BSS algorithm refers to the process of separating various source signals from the observed signal when the theoretical model of the source signal is unknown and obtaining the best estimation of the source signal model and signal amplitude. When applying the BSS algorithm to NMR data processing, the laboratory and downhole NMR data can be considered as the observed signal, the relaxation components with specific NMR response can be considered as the source signal, and the proportions of different relaxation components can be considered as the signal amplitude. Based on the BSS algorithm, NMR responses and proportions of different components can be obtained.

We applied the BSS algorithm to the laboratory and downhole NMR data. Four pore types with different pore radius can be discriminated and their proportion can be extracted from the laboratory and downhole NMR data. The permeability of tight sandstone formation is affected by many factors and has poor correlations with the porosity. Based on the thin section observation, MICP and NMR analysis, the pore space of tight sandstone formation is complex and can be divided into micropore, mesopore, macropore and megapore. Pore structure is one of the main influential factors of permeability in tight sandstone formations. Relaxation components with the same NMR response and their proportions can be extracted from the BSS algorithm. Four relaxation components referring to different pore types can be obtained from laboratory and downhole NMR data. The permeability of tight sandstone formation is positively correlated with proportions of macropore and megapore, while negatively correlated with proportions of micropore and mesopore. A new permeability estimation method is established based on porosity, geometrical T2 value, the sum proportion of macropore and megapore, and the sum proportion of micropore and mesopore. The new model achieves great results compared with the conventional models. The new method can be easily extended in other tight sandstone formations where the main influential factors of permeability are porosity and pore structure. Besides, laboratory experiments and core calibration can significantly improve the accuracy of permeability estimation.

How to cite: Liu, J.: A new permeability estimation method based on blind source separation and NMR data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18330, https://doi.org/10.5194/egusphere-egu25-18330, 2025.

EGU25-19812 | ECS | Posters on site | GI5.4 | Highlight

A holistic approach to low-field NMR and MICP data integration for the accurate determination of the absolute pore size distribution in siliciclastic rocks 

Michał Fajt, Grzegorz Machowski, Bartosz Puzio, and Artur Tadeusz Krzyżak

Low-field nuclear magnetic resonance (LF-NMR) has emerged as a critical tool in geophysical prospecting, particularly for reservoir rocks exploration and their pore space characterization. However, accurate assessment of pore size distribution (PSD) in unconventional reservoirs, such as tight sandstone and shale formations, remains challenging due to their complex pore structures, high clay mineral content, low porosity, and nanometer-scale pore sizes. Additionally, these challenges can be further amplified by the presence of internal gradients (G), induced by differences in magnetic susceptibility of the rock matrix and saturating fluid, which can distort PSD estimates obtained under traditional assumptions of their negligibility.

In the fast diffusion regime, as demonstrated by Brownstein and Tarr, NMR transverse relaxation time (T2) is proportional to pore size, with the proportionality factor governed solely by surface relaxivity (ρ2). However, conventional approaches assume negligible internal gradients which often lead to unrealistic PSD results, especially in nanometer-scale pores where the induced gradient effect can be significant. Internal gradient is inversely proportional to the pore size and can cause substantial distortions even when applying low field and CPMG sequence with low echo times (TE) in rocks of minimal paramagnetic mineral content.

This work presents a novel methodology integrating differential LF-NMR with mercury injection capillary pressure (MICP) for simultaneous estimation of PSD, ρ2, and internal gradients in siliciclastic reservoir rocks. This approach enables comprehensive evaluation of pore space, accounting for both ρ2 and internal gradients without requiring additional magnetic susceptibility measurements. LF-NMR relaxometry was conducted on rock core samples saturated with kerosene having a bulk self-diffusion coefficient almost three times lower compared to water to minimize the effects of diffusion in nanopores and stay within detection limits for this pore size range, as well as to preserve samples from dissolving. ρ2 and G were estimated based on the specific conversion framework established using physical characteristics of the kerosene molecule, percolation theory and non-linear PSD–T2 transformation.

The methodology was applied to core samples from various lithologies, including sandstones, heteroliths, and mudstones of wide pore size ranges, offering insights into the interplay of ρ2 and internal gradient influence over PSD across diverse siliciclastic rock matrices.

Preliminary findings demonstrate that the differential LF-NMR protocol effectively identifies open-pore space systems while mitigating the influence of clay minerals and organic matter on PSD estimates. Furthermore, by incorporating ρ2 and internal gradient effects on T2 relaxation, our approach provides realistic PSD values, covering the open-pore size range down to 0.6 nm, the smallest particle diameter of kerosene. Validation of obtained PSD was additionally conducted through nitrogen (N2) adsorption measurements. Importantly, it is planned to develop empirical LF-NMR PSD models that can overcome the limitations of traditional destructive MICP and nitrogen adsorption methods in detecting pores in siliciclastic rocks with diameters below 3 and 1.78 nm, respectively.

How to cite: Fajt, M., Machowski, G., Puzio, B., and Krzyżak, A. T.: A holistic approach to low-field NMR and MICP data integration for the accurate determination of the absolute pore size distribution in siliciclastic rocks, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19812, https://doi.org/10.5194/egusphere-egu25-19812, 2025.

Polycyclic aromatic hydrocarbons (PAHs) are a group of toxic organic pollutants that originate from the incomplete combustion of organic matter. Due to lipophilic and hydrophobic properties, PAHs tend to be adsorbed by soil particles. Source apportionment of soil-bound PAHs contributes to controlling emissions and protecting the ecological environment. This research investigated source and distribution characteristics of PAHs in soils from Campania region of Italy, especially the natural sources. The total PAH concentrations ranged from N.D. to 4191 ng/g soil (dry weight). The data do not follow either a normal or lognormal distribution, but rather absolutely the multifractal distribution. Spatially distributed PAHs have experienced different degrees of superposition on the basis of multifractal spectrums curves with asymmetric upper convex. In addition, multifractal spectrum curves are all in a right hook shape, representing that low-values are dominant in the Campania area. The local singularity analysis shows an enrichment phenomenon that is not identified by the spatial interpolation method. The singularity values of PAHs were significantly correlated with TOC, but not significant with pH and population density. As opposed to concentrations, singularity indexes mainly reflecting the influence of soil properties. The fractal method was successfully used to separate the natural sources from the anthropogenic contributions of PAHs. Our results indicate that PAHs mixing distributions may be decomposed into natural background, anthropogenic background, and point source pollution. The background field was attributed to the thermal effects of geological processes, whereas anthropogenic anomaly was associated with anthropogenic activities. In sum, our study provides evidence of natural sources evidence that volcanic events have key effects on the distribution of PAHs, and shows that anthropogenic sources of PAHs are related to regional industrialization and urbanization status.

How to cite: Shi, C. and Qu, C.: Decoupling natural and anthropogenic polycyclic aromatic hydrocarbons in the soil environment, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2421, https://doi.org/10.5194/egusphere-egu25-2421, 2025.

EGU25-6105 | Orals | GI5.5

Determination of geochemical background/baseline values in a biogeochemical province (a case study of the Lori region, Armenia) 

Gevorg Tepanosyan, Zhenya Poghosyan, Astghik Gevorgyan, Karine Davtyan, and Lilit Sahakyan

The geochemical background/baseline is a key parameter for assessing environmental contamination and identifying potential risks to ecosystems and human health. However, the determination of these values requires careful handling of geochemical data. In practice, the geochemical background of chemical elements can be determined by both empirical and geostatistical methods. In addition, depending on the sampling scale and the area's natural landscape-geochemical characteristics, especially in biogeochemical provinces, the use of a single approach can lead to bias. Therefore, combining both approaches and incorporating several methods of geochemical data processing and spatial clustering is needed to unveil the hidden patterns and delineate representative areas, where separate processes and factors (natural and anthropogenic) condition the contents and distribution of chemical elements. In addition, adding auxiliary information related to the geological setting, soil types and potential sources of contamination can ensure the refinement of the data processing and increase the reliability of the estimated background/baseline values. This study aims to determine the geochemical background/baseline of arsenic (As) in the Lori region (Armenia) by dividing the soil data set into homogeneous subsamples using an algorithm combining data transformation, hot spot analysis (Local Moran I), univariate outlier detection and concept of normal distribution. The results of the study showed that the application of the Local Moran I index allows to identify clusters of samples (of high-high (HH) values, low-low (LL) values and not-significant (NS) values) that have a clear spatial separation. The boxplots of the As contents in the identified subsamples showed that outliers and extreme values are presented. After the elimination of these values, normal distribution was confirmed (Shapiro-Wilk test). The median value of As was 13 mg/kg, 16 mg/kg and 24 mg/kg for LL, NS and HH values, respectively. Meanwhile, the 95 percentile of the LL and NS values were 16 mg/kg and 21.4 mg/kg, respectively. The cluster of HH values spatially covers an area known for its natural mineralization, mining sites and Cu smelter, implying some level of anthropogenic quantities of As which is superimposed on the natural contents. Therefore, the estimated value for this area can be considered as a geochemical baseline rather than a geochemical background. The results of this study showed that in the case of biogeochemical provinces where natural mineralization and anthropogenic activities are presented, several background/baseline values can be determined. The algorithm proposed in this study can be used for other elements and serve as a justified approach to separate homogeneous subsamples and delineate areas for the application of these reference values.

How to cite: Tepanosyan, G., Poghosyan, Z., Gevorgyan, A., Davtyan, K., and Sahakyan, L.: Determination of geochemical background/baseline values in a biogeochemical province (a case study of the Lori region, Armenia), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6105, https://doi.org/10.5194/egusphere-egu25-6105, 2025.

Many environmental and geological phenomena are inherently complex, shaped by the interplay of physical, chemical, biological, and anthropogenic factors. These interactions often result in spatial asymmetries, where high and low values exhibit distinct statistical behaviors. For instance, a contaminant field may simultaneously reflect natural and anthropogenic sources, producing unique spatial patterns that challenge conventional analysis.

Despite significant advancements in geostatistics, multivariate spatial models remain limited. The linear model of coregionalization (LCM) dominates the field but assumes symmetrical dependencies and Gaussian behavior. These assumptions restrict its ability to capture the structural complexity of multivariate spatial data, potentially obscuring meaningful relationships or introducing misleading correlations.

This presentation introduces a stochastic methodology for simulating non-Gaussian multivariate random fields using a non-linear model of coregionalization (N-LCM). The proposed approach accounts for rank asymmetry (differing spatial dependencies for low and high values) and directional asymmetry (variations in spatial dependence across directions). It supports multiple dependencies between variables, allowing some to exhibit Gaussian behavior while others display non-Gaussian characteristics. Pseudo-admissible N-LCMs are approximated through spectral decomposition, with negative eigenvalues replaced by zero.

The methodology leverages an adapted Generalized Fast Fourier Transform Moving Average (G-FFTMA) algorithm for multivariate non-Gaussian geostatistical simulations, offering a flexible and efficient framework for analyzing and simulating complex datasets. Synthetic examples demonstrate the method’s ability to uncover meaningful spatial patterns. Additionally, a real-world case study highlights the duality between natural contamination and anthropogenic emissions from a smelter in Quebec, Canada. This case study emphasizes the methodology’s capability to analyze geochemical processes influenced by human activities and environmental interactions.

This research advances geostatistics and multivariate analysis, providing new insights into geological and environmental processes at the Earth’s surface.

How to cite: Lauzon, D., Hörning, S., and Bárdossy, A.: A Novel Framework for Stochastic Simulation of Multivariate Non-Gaussian Random Fields in Environmental and Geological Studies, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7198, https://doi.org/10.5194/egusphere-egu25-7198, 2025.

EGU25-7643 | ECS | Orals | GI5.5

A new approach to evaluate hydrocarbon generation characteristics by pyrolysis Tmax in lacustrine shale oil plays 

Shengnan Liu, Shiju Liu, David Misch, Xiangyun Shi, Congsheng Bian, Wenzhi Zhao, and Rukai Zhu

It has been revealed that significant disparities in both the organic matter source and hydrocarbon generation characteristics of lacustrine sedimentary environments, causing challenges in the assessment of continental shale oil prospects  . Lacustrine-sourced shale oil resources in China exhibits notable longitudinal and vertical heterogeneity, which poses a substantial challenge in objectively assessing geological resources and shale oil prospects, especially in a region characterized by overall low thermal evolution . Advanced pyrolysis or bulk kinetic experiments are invaluable tools to refine the understanding of petroleum generation timing . Nevertheless, such experiments are expensive and time-consuming and hence cannot be executed on extensive sets of samples to capture the overall lateral and vertical variability that a source formation may inherit  .In this study, we proposed a new method to rapidly evaluate the hydrocarbon generation characteristics of lacustrine source rocks utilizing anomalies in the Rock-Eval pyrolysis parameter Tmax across various lacustrine shales.

The workflow is depicted as flows: The analysis workflow starts with the selection of samples with TOC exceeding 1 wt.%, given the economic exploration potential of these shales. Subsequently, these samples are categorized into low and high maturity profiles based on the measured vitrinite reflectance (Ro). The two maturity profiles are further classified into low and high Tmax classes using machine learning data analysis. The kmeans clustering method in the Python library scikit-learn was utilized to classify different Tmax values to specific classes  . In certain instances, a third cluster or class may be necessary, depending on the data structure. Samples in the “low Tmax” class typically exhibit high Production Index (PI = S1/(S1+S2)) while the Hydrogen Index (HI: = S2/TOC*100) values decrease with increasing maturity. In contrast, the “high Tmax” class maintains consistently high HI and low PI at different maturity levels. This analysis workflow facilitates the identification of distinct hydrocarbon generation characteristics for source rocks at different maturity levels based on the Tmax values.

Overall, the “low Tmax” class shows characteristics of early hydrocarbon generation, low activation energy, and wide hydrocarbon generation windows, while the “high Tmax” class shows characteristics of late hydrocarbon generation, high activation energy, and narrow hydrocarbon generation windows. Notably, these diverse hydrocarbon generation characteristics are mainly related to the composition of the primary organic matter, a correlation that can be confirmed through organic petrographical observations.

This analysis workflow is validated with three examples. There are a great data pool of Tmax,and it is recommended to shift the focus towards source rocks that host organic matter favorable for early oil generation. This involves identifying rocks with low Tmax values and hence low activation energy, as they are indicative of conditions conducive to the initiation of oil generation. When it comes to in-situ heating, The exact prediction of hydrocarbon generation processes enables a more precise calculation of current geological recoverable resources. This study has important guiding significance for oil and gas exploration.

Fig. 1. Workflow for determining hydrocarbon generation characteristics of source rocks by a classification according to Tmax variability.

How to cite: Liu, S., Liu, S., Misch, D., Shi, X., Bian, C., Zhao, W., and Zhu, R.: A new approach to evaluate hydrocarbon generation characteristics by pyrolysis Tmax in lacustrine shale oil plays, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7643, https://doi.org/10.5194/egusphere-egu25-7643, 2025.

The traditional kinetic model reflects the impact of fixed pressure on hydrocarbon generation in thermal simulation experiments, but the pressure in experiments differs from the overpressure in formation, affecting the evaluation of hydrocarbon generation. In this study, a new parallel first-order reaction kinetic model for hydrocarbon generation in relation to formation overpressure retardation is proposed and its application is illustrated.

According to the impact of pressure on activation energy (E) and pre-exponential factor (A), the pressure factor is introduced into the Arrhenius formula:

k=exp(p/a)·exp⁡(-(np+E)/RT)

Where k is the reaction rate at 1 bar, R is the universal gas constant, T is the absolute temperature (K), p is pressure (MPa), a and n are the impact factors of pressure on A and E respectively.

By calculating n and a, the new model can simulate hydrocarbon generation under any temperature and pressure and is no longer limited by experimental conditions.

Sample from Baiyun Depression in the Pearl River Mouth Basin were selected to carry out a gold-tube thermal simulation, and the kinetic parameters of natural gas generation were calculated by using the new model. Since the traditional model reflects the impact of experimental pressure, the new model calculates the kinetic parameters without the impact of pressure, therefore, the average activation energy (Ea) calculated by the traditional model is greater than that of the new model, and the impact of pressure is reflected by impact factors (n and a)(Fig. 1).

Figure 1 Comparison of kinetic parameters of natural gas generation calculated by traditional model and new model

Figure 1 Comparison of kinetic parameters of natural gas generation calculated by traditional model and new model

The new model reflects the inhibition effect of overpressure on natural gas generation (Fig. 2). According to the information on fluid inclusions, The kerogen began to generate mass gas at 23 Ma. The calculation results of the traditional model show that kerogen starts to enter the large-scale gas generation stage at 32 Ma, which is inconsistent with the time of overpressure formation. When the formation pressure coefficient is 1.8, the mass hydrocarbon generation time calculated by the new model is about 24 Ma, which is more consistent with the geological reality. The new model proves that natural gas generation is retarded under the impact of overpressure.

Figure 2 Comparison of the conversion rate of natural gas of the traditional model and the model in relation to overpressure under geological conditions.The black line reflecting the influence of pressure under experimental conditions; the blue line is the history of natural gas generation without the impact of overpressure; the orange line is the history of hydrocarbon generation under formation overpressure.

Figure 2 Comparison of the conversion rate of natural gas of the traditional model and the model in relation to overpressure under geological conditions.The black line reflecting the influence of pressure under experimental conditions; the blue line is the history of natural gas generation without the impact of overpressure; the orange line is the history of hydrocarbon generation under formation overpressure.

How to cite: Jiang, J. and Li, J.: Overpressure retardation of hydrocarbon generation: a new kinetic model considering the effects of pressure and its application, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8179, https://doi.org/10.5194/egusphere-egu25-8179, 2025.

Qinghai Province, in northwest China's low-density population areas, is known for its high-altitude landscape and abundant surface water. This study investigates 48 sediment samples from 19 quintessential plateau lakes distributed in the Qilian Mountains, Qaidam Basin, Yellow River source regions, and Yangtze River source regions of Qinghai Province, focusing on 7 potentially toxic elements (PTEs ) and 16 priority polycyclic aromatic hydrocarbons (PAHs). Compared to other plateau lake sediments domestically and internationally, concentrations of PTEs ( Ni, Zn, Pb, Cu, Cr, Co, and As) and PAHs (Nap, Acy, Ace, Flu, Phe, Ant, Fla, Pyr, BaA, Chr, BbF, BkF, BaP, IcdP, DahA, and BghiP) in the studied sediment samples were relatively low. Spatial distribution characteristics of PTEs and PAHs contents show that the similar trend between the four regions was like that: Qaidam Basin> Yangtze River source>Yellow River source> Qilian Mountains. Additionally, positive matrix factorization (PMF) and species sensitivity distributions (SSD) are employed  to assess pollution source levels and ecological risks in the study lake regions,respectively.The study reveals that the total average concentrations of PTEs and PAHs in the sediments of the 19 Qinghai lakes were individually 132.93 mg/g and 27.64 ng/g,  which were quite low compared to lake sediments in other plateau regions both domestically and internationally. PMF analysis identified fisheries, animal husbandry, mining, rock weathering, and agriculture as PTE sources.While oil leakage, combustion, and auto emissions were identified as PAH sources. It is found that SSD-based health risk assessment shows the risks was far below the acceptable threshold (0.1). However, the highest risks were concentrated mainly in the downstream areas of the estuaries and near tourist and agricultural sites, such as the studied sites in Keluke Lake (Qaidam Basin), Eling Lake (Yellow River source region), and Tuosu Lake (Qaidam Basin). Notably, Cu, As, and Phe exhibited higher ecological risk indices. In general, despite the current research indicating low and negligible health risks posed by PTEs and PAHs in these plateau lakes, it is necessary to keep monitoring and controlling to prevent any escalation of ecological risks in the fragile lake environment.

How to cite: Sun, W., Zhang, J., Wang, W., and Qu, C.: Sources apportionment and ecological risk assessment of potentially toxic elements (PTEs) and polycyclic aromatic hydrocarbons (PAHs) in surface sediments of plateau Lakes of Qinghai Province, China, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10689, https://doi.org/10.5194/egusphere-egu25-10689, 2025.

EGU25-12283 | Orals | GI5.5

Geostastical modeling of space-time dynamics calcite dissolution at the nanoscale 

Emmanouil Varouchakis, Chiara Recalcati, Laura Ceresa, Monica Riva, and Alberto Guadagnini

We investigate the intricate patterns associated with space-time dynamics displayed by (i) surface topography (Z) and (ii) reaction rates (R) resulting from direct nano-scale imaging of calcite-water interfaces subject to dissolution. The analysis rests on a space-time variogram modeling approach. The latter has been suggested as promising in unveiling major patterns exhibited by hydrogeological quantities across large scale aquifer systems. Transferability of the associated theoretical and operational framework to interpret nano-scale geochemical scenarios is here assessed for the first time. We do so upon taking advantage of recent high-resolution experiments attained through Atomic Force Microscopy (AFM) and targeting the evolution of the interface between a calcite crystal and water as driven by mineral dissolution processes. Upon relying on the ensuing large data-set, key variability patterns are identified through (i) efficient sampling of the spatial domain via quasi-random Sobol sequences and (ii) the use of a Harmonic Covariance Estimator (HCE) to model the space-time variogram of Z. The resulting (sample) space-time variogram exhibits visibly periodic oscillations at specific spatial and temporal lags. These patterns highlight the interaction taking place between the spatial structure and temporal dynamics in hydrogeological processes. We also explore the theoretical bases of the relationship between the variograms of Z and R. Corresponding results offer valuable insights into the spatial and temporal correlation of calcite dissolution dynamics. Our findings enable one to link space-time dynamics of crystal topography and the ensuing dissolution rates to corresponding traits of space-time variograms. Hence, they constitute the basis for potential applications associated with the possibility of providing estimates of the way these complex processes evolve at nano-scale resolutions, thus driving chemical weathering of minerals constituting the Earth’s interior.

 

How to cite: Varouchakis, E., Recalcati, C., Ceresa, L., Riva, M., and Guadagnini, A.: Geostastical modeling of space-time dynamics calcite dissolution at the nanoscale, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12283, https://doi.org/10.5194/egusphere-egu25-12283, 2025.

EGU25-12634 | ECS | Orals | GI5.5

Hydrogeochemical characterization and assessment of groundwater quality in Muyira Sector, Rwanda. 

Emmanuel Ngendahayo, Melab Impuhwezayo, Emmanuel Nkurunziza, and Jean Nepo Nsengiyumva

The Muyira sector is one of ten sectors of the Nyanza district in the Amayaga region of Rwanda. Amayaga region is part of the country's drought-prone areas, with high groundwater dependence. Most inhabitants in the area depend on groundwater for drinking and domestic purposes. Therefore, a hydrogeochemical characterization and assessment of groundwater quality in the study area was carried out using a combined application of hydrochemical models, multivariate statistical techniques, and GIS-based ordinary kriging interpolation on seven (7) borehole water samples. This study aimed to determine the concentrations and spatial distribution of various ions, groundwater quality issues, and the geochemical processes contributing to groundwater chemistry. The abundance of major cations in the groundwater is in the order Na+ > Ca2+ > K+ > Mg2+, whereas that of the major anions varies in the order HCO3 > SO42− > Cl. Ca-Mg-Na-HCO3 water type is common in the area, possibly due to the dissolution of magnesite and silicate minerals in the basement rocks. Also, results indicate weak acids (i.e., HCO3) dominance over strong acids (i.e., SO42− and Cl). Ion exchange reactions and magnesite and silicate minerals weathering primarily control the area's groundwater chemistry. The results of the Pollution Index for Groundwater (0.29-0.55) and Groundwater Quality Index (29.14-53.68) indicate groundwater in the area is suitable for drinking. The sodium percentage (36.88–78.20%, mean of 57.83%), magnesium ratios (13.90–94.66, mean of 35.70), and sodium adsorption ratio (4.63–16.92, mean of 11.78) suggests that groundwater in the study area is suitable for irrigation purposes.

How to cite: Ngendahayo, E., Impuhwezayo, M., Nkurunziza, E., and Nsengiyumva, J. N.: Hydrogeochemical characterization and assessment of groundwater quality in Muyira Sector, Rwanda., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12634, https://doi.org/10.5194/egusphere-egu25-12634, 2025.

EGU25-12894 | ECS | Orals | GI5.5

Applying fingerprinting methods on multielement measurements to track sediment transport in a small erosion-prone hilly catchment 

Máté Krisztián Kardos, Zsolt Jolánkai, and Adrienne Clement

To investigate particulate material dynamics,  48 soil, river bottom sediment, and river suspended particulate matter (SPM) samples were collected using a stratified sampling method in the Koppány River Basin, Hungary. Samples were analyzed via inductively coupled plasma mass spectrometry for the concentration of 44 elements, encompassing heavy metals, "light" metals, and rare earth elements. Multivariate statistical methods, particularly hierarchical cluster analysis and principal component analysis (PCA) were applied to identify patterns and drivers of material distribution across the catchment.

The PCA results revealed distinct partitioning of particulate material sources and transport behaviors. The first principal component (PC1) distinguished SPM samples from soil and sediment samples, underscoring the contrasting geochemical signatures of material mobilized during different flow conditions. The second principal component (PC2) separated SPM samples collected during low flow conditions from those collected during high flow conditions, reflecting hydrological influences on particulate transport and source contributions. Notably, spatial differences between the upper and lower parts of the catchment were found to be less significant than the temporal dynamics driven by flow conditions.

These preliminary findings highlight the pivotal role of hydrology in governing the geochemical composition of suspended materials and provide insights into sediment dynamics in hilly river basins. The study demonstrates the utility of multivariate approaches in disentangling complex interactions between geological and hydrological processes in catchment systems.

How to cite: Kardos, M. K., Jolánkai, Z., and Clement, A.: Applying fingerprinting methods on multielement measurements to track sediment transport in a small erosion-prone hilly catchment, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12894, https://doi.org/10.5194/egusphere-egu25-12894, 2025.

EGU25-16437 | Posters on site | GI5.5

The application of Principal Component Analysis to reveal the contributions of various natural and anthropogenic sources to the chemical composition of soil. 

Antonio Iannone, Chaosheng Zhang, Annalise Guarino, Alessio De Falco, Lucia Rita Pacifico, and Stefano Albanese

Environmental risks are often linked to contamination processes driven by various chemical stressors introduced into the environment from specific sources. These sources may be anthropogenic, stemming from human activities, or natural, associated with the geolithological context and geological weathering processes. It is crucial to distinguish between chemical anomalies resulting from anthropogenic inputs and those arising from the inherent compositional characteristics of the natural environment, which may not be remediable. This differentiation is essential for establishing reliable and practical remediation objectives.

When anthropogenic activities release waste products into the environment in airborne, liquid, or solid forms, these materials typically possess distinct chemical compositions. Such compositions frequently involve associations of substances that can disrupt environmental equilibria. This study employed both univariate and multivariate statistical techniques to analyze geochemical data from over 7,000 topsoil samples collected in the Campania region of Southern Italy. The objective was to develop an operational model for assessing environmental risks by identifying their sources. The database encompasses the concentrations of 52 chemical elements for each sample, with data georeferenced to facilitate spatial analysis, delineate geochemical patterns, and correlate anomalies with known human or natural sources.

The complex geological setting of the Campania region, combined with the diverse sources of anthropogenic contamination, rendered Principal Component Analysis (PCA) an especially effective method for identifying element associations that predominantly influence the variability of the geochemical data. PCA was conducted using a selection of 21 variables, resulting in the identification of four significant principal components (PCs) that account for the majority of the observed data variability:

- PC1 (42% of total variance), characterized by Th, Be, As, U, V, and Bi.

- PC2 (16% of total variance), characterized by Sb, Zn, Hg, Pb, Sn, and Cd.

- PC3 (10% of total variance), characterized by Mn, Ni, Cr, and Co.

- PC4 (9% of total variance), characterized by Ba, Cu, and Sr.

The scores of the components for each sample were spatially plotted and classified to enhance their interpretability. The legend for the component scores was centered at zero, indicating the minimal contribution of the covered areas to overall component variability; higher absolute values identified areas where the featured elemental association was more significant.

The analysis effectively differentiated soils predominantly influenced by natural contributions, such as loose materials from the volcanic centers of Campania (e.g., Mt. Roccamonfina, Campi Flegrei, and Mt. Somma-Vesuvius) (PC1 and PC4) and weathering products from the region's siliciclastic deposits (PC3). Furthermore, the PCA found areas subjected to considerable anthropogenic pressure concerning the association of Sb, Zn, Hg, Pb, Sn, and Cd (PC2). These findings underscore the effectiveness of multivariate analysis, particularly PCA, in discriminating between geogenic and anthropogenic processes and, further, in distinguishing among various anthropogenic sources. This methodological approach offers valuable insights for managing environmental risks and prioritizing remediation efforts.

How to cite: Iannone, A., Zhang, C., Guarino, A., De Falco, A., Pacifico, L. R., and Albanese, S.: The application of Principal Component Analysis to reveal the contributions of various natural and anthropogenic sources to the chemical composition of soil., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16437, https://doi.org/10.5194/egusphere-egu25-16437, 2025.

EGU25-17328 | Orals | GI5.5

Hotspot analysis for discriminating geochemical anomalies in the soil of an intensely anthropized volcanic region in Italy. 

Stefano Albanese, Antonio Iannone, Chaosheng Zhang, Annalise Guarino, Alessio De Falco, and Lucia Rita Pacifico

Soils result from physical, chemical, and biological processes that affect rocks and their weathered products. In historical times, natural processes have also been widely influenced by human activity (such as industrial production, motor vehicle mobility, waste disposal, and agricultural practices). Consequently, soils represent a reservoir of chemical elements and compounds with extreme spatial variability across Earth's surface.

Defining the distribution of chemical elements and their anomalies and understanding the nature of factors controlling their spatial variability is essential for those committed to environmental issues management, especially when effects on ecosystems and living beings must be addressed, targeting the development of remedial actions.

In recent years, with the rapid data volume growth, effective methods are required for data analytics for large geochemical datasets. Spatial machine learning technologies have been proven to have the potential to reveal hidden patterns based on geochemical information. In this study, a spatial clustering technique of Getis-Ord Gi* statistic was performed on 21 characterizing elements using more than 7000 topsoil samples (~ 7300) proceeding from the Campania region territory in southern Italy.

The analysis found spatial clusters of significantly high (hot spots) and low values (cold spots) for the selected elements, showing a strong correlation with the geological features of the study area, particularly volcanic and siliciclastic units.

Volcanic units were associated with high concentrations of elements such as As, Ba, Be, Bi, Cu, Sr, Th, Tl, U, and V, while siliciclastic units were associated with high values of Co, Cr, Ni, and Mn. Additionally, the high concentration of Cd, Hg, Pb, Sb, Sn and Zn showed a clear association with the region's main urban and industrial centres.

The results highlight the power of spatial clustering techniques in discriminating geogenic from anthropogenic processes and identifying hidden spatial patterns, thus offering valuable insights for environmental studies and management.

How to cite: Albanese, S., Iannone, A., Zhang, C., Guarino, A., De Falco, A., and Pacifico, L. R.: Hotspot analysis for discriminating geochemical anomalies in the soil of an intensely anthropized volcanic region in Italy., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17328, https://doi.org/10.5194/egusphere-egu25-17328, 2025.

EGU25-17982 | Posters on site | GI5.5

Harnessing soil geochemistry and granulometry for optimal terroir management and wine profiling: insights from the Taurasi terroir of southern Italy 

Domenico Cicchella, Maurizio Ambrosino, Ilaria Guagliardi, and Stefano Albanese

The interaction between the unique geochemical characteristics of the soils and the social, environmental, climatic and biodiversity factors give distinctive properties to the wines of a specific area, defining the terroir of a wine. While climatic, ecological, and social aspects remain relatively stable within the limited extension of terroirs, soil geochemistry can change notably. Variations in soil geochemistry play a significant role as they influence vine health, grape quality and, ultimately, the flavour profile of the wine. This study aims to highlight the chemical and granulometric differences occurring in the Taurasi terroir (Southern Italy) to improve its management and enhance the diverse flavours and aromas of the wines. The Taurasi terroir encompasses an area of 245 km², within which soils belong to three different geochemical domains (clay, volcanic, and carbonate soils). Chemical elements affecting colour and aroma (Cu, Fe), taste (Na, K), metabolism and photosynthesis (B, Mn, Zn), or potentially toxic elements for vines (Al, As) were analysed in 100 topsoil samples distributed across the three geochemical domains. Additionally, granulometry and organic carbon content were also analysed to assess soil's ability to retain water and microbial populations. Results revealed significant compositional differences among the three geochemical domains that inevitably reflect in wine characteristics. Except for Mn, volcanic soils were enriched in all analysed elements, while carbonate soils were depleted. Following the order of volcanic soils – clay soils – carbonate soils, the average concentrations of analysed elements were as follows: As (16 - 7 - 3 mg/kg); Al (5.5 - 3.2 - 1.8 %); B (24 - 10 - 6 mg/kg); Cu (78 - 52 - 28 mg/kg); Fe (3.2 - 2.7 - 1.8 %); K (1.6 - 0.7 - 0.4 %); Mn (950 - 1470 - 820); Na (0.6 - 0.05 - 0.05 %); Zn (105 - 62 – 58 mg/kg). From a granulometric perspective, volcanic soils were coarse-grained, followed by carbonate and clay soils. The average granulometry for the three geochemical domains is as follows: volcanic soils (72% sand, 13% silt, 5% clay); carbonate soils (26% sand, 58% silt, 16% clay); clay soils (5% sand, 13% silt, 72% clay). Average organic carbon values were also favourable for volcanic soils (4.5%), followed by carbonate soils (3.2%) and clay soils (1.4%). These results show that significant compositional and granulometric differences within the Taurasi terroir are reflected in the expression of grapes and wines produced. Therefore, this study provides key tools for micro-zoning terroirs to enhance diverse flavour, colour, and aroma expressions within the same terroir.

How to cite: Cicchella, D., Ambrosino, M., Guagliardi, I., and Albanese, S.: Harnessing soil geochemistry and granulometry for optimal terroir management and wine profiling: insights from the Taurasi terroir of southern Italy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17982, https://doi.org/10.5194/egusphere-egu25-17982, 2025.

EGU25-18176 | ECS | Orals | GI5.5

The role of soil geochemistry in the absorption of potentially toxic elements (PTEs) by edible hyperaccumulator plants: the case of Brassica rapa in volcanic and clay soils. 

Maurizio Ambrosino, Giuseppe Diego Puglia, Eleonora Maria Di Salvo, Shashank Saini, Nicola Cicero, and Domenico Cicchella

The hyperaccumulation behaviour of PTEs is observed in many edible plants. However, the role of soil geochemistry and the human health risks associated with the uptake of PTEs by hyperaccumulator plants remain poorly understood. This study analyses 10 topsoil and Brassica rapa samples collected from volcanic and clay soils, comparing the contents of As, Cd, Hg and Pb and assessing their relative health risks. To account for geochemical variations in volcanic and clay soils, samples were collected from two Italian regions (Sicily and Campania) characterized by different geological settings. The results indicate that volcanic soils exhibit higher concentrations of PTEs than clay soils, with Hg levels exceeding precautionary limits established by EU soil quality standards. Notably, Campania shows the highest concentrations of PTEs in soils, attributable to evolved magmatic products with tephritic-phonolitic composition. In clay soils, Sicilian samples reveal significant enrichment in Cd, while As, Hg and Pb are more concentrated in Campanian clays. Soil quality standards are not exceeded in clay soils. Regarding plant tissues, concentrations of Cd, Hg and Pb in edible organs (stems and leaves) exceed FAO-WHO standards in most samples from volcanic soils, with values up to 3, 8, and 14 times higher than the standards. Plants grown in clay soils show lower concentrations of PTEs than those grown in volcanic soils; only one Sicilian sample exhibits concentrations of Cd, Hg, and Pb 4, 1.5, and 6 times above FAO-WHO standards, respectively. The bioconcentration factor (BCF) and translocation factor (TF) confirm the hyperaccumulating behaviour of Brassica rapa, with concentrations of PTEs in roots and stems sometimes exceeding those present in the soil. Risk analysis revealed that total cancer risk and target hazard quotient are unacceptable for adults and children who consume Brassica rapa from volcanic soils. Both parameters generally show acceptable values in clay soils, with alarming levels only for high consumption rates. Finally, although Sicilian soils are generally impoverished in PTEs, Brassica rapa samples from this region exhibit higher levels than those from Campania. Therefore, while soil geochemistry is a crucial factor in metal absorption by Brassica rapa, other parameters (e.g., climatic, environmental, and biological) also play a significant role.

How to cite: Ambrosino, M., Puglia, G. D., Di Salvo, E. M., Saini, S., Cicero, N., and Cicchella, D.: The role of soil geochemistry in the absorption of potentially toxic elements (PTEs) by edible hyperaccumulator plants: the case of Brassica rapa in volcanic and clay soils., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18176, https://doi.org/10.5194/egusphere-egu25-18176, 2025.

EGU25-18593 | ECS | Posters on site | GI5.5

Environmental Distribution and Source Analysis of Organochlorine Pesticides in the Soils of the Sarno River Basin, Southern Italy 

Annalise Guarino, Antonio Iannone, Alessio De Falco, and Stefano Albanese

The Sarno River Basin (SRB) is among the most polluted in Europe, with contamination deriving from industrial activities, including tanneries and canneries, as well as intensive agriculture and dense urbanization. It is located in the Campania region in Southern Italy, in the southwestern portion of the Campania Plain, between the Somma–Vesuvius volcanic complex to the west and the Lattari Mountains carbonate reliefs to the south.

The SRB is characterized by the presence of high concentrations of some priority organic pollutants, deriving from their use in various processes linked to human activities (e.g., agriculture, industry, mining, vehicular traffic). The soils of the basin, predominantly fine-grained alluvial and volcanic deposits, provide an ideal matrix for the retention of these pollutants, further enhanced by the high organic matter content.

Organochlorine pesticides (OCPs) are synthetic organic compounds extensively utilized in agriculture as insecticides and fungicides during the mid-20th century and, subordinately, in the medical field. These chemicals are among the most common soil contaminants, especially in highly industrialized and anthropized areas; they show a high environmental persistence and are generally characterized by a marked tendency towards bioaccumulation and biomagnification along trophic chains due to their lipophilic character.

The study aims to assess the geochemical-environmental conditions of the SRB, through GIS-based maps and univariate statistical analysis, also establishing the nature of their potential emission sources. For the purpose, over an area of about 500 km2 a total of 42 topsoil samples were collected to be analyzed to determine the concentration levels of 24 OCPs.

To investigate the distribution pattern of concentrations, the compounds were grouped into six classes:

  • I) dichloro-diphenyl-trichloroethane (DDT) and its isomers and metabolites (DDE, DDD), whose Ʃ6DDTs concentrations represent on average 68.7% of the total OCPs and ranges from a minimum of 0.021 µg/kg to a maximum of 339 µg/kg;
  • II) hexachlorocyclohexane (HCH) isomers (α, β, γ, δ), with Ʃ4HCHs representing 2.64% and ranging from 0.013 µg/kg to 7.84 µg/kg;
  • III) aldrin, dieldrin, and endrin, whose Ʃ3Drins varies from 0.010 µg/kg to 71.7 µg/kg and constitutes the 6.61%;
  • IV) heptachlor, chlordane (α, γ), and nonachlor (cis, trans), constituting on average 1.39% with Ʃ5Chlors from 0.016 µg/kg to 0.94 µg/kg;
  • V) Endosulfan (α, β), and Endosulfan sulfate, whose Ʃ3Endos varies from 0.010 µg/kg to 19.3 µg/kg and represents 14.5%;
  • VI) mirex, methoxychlor and hexachlorobenzene, constituting 6.18%, with total values from 0.010 µg/kg to 7.01 µg/kg.

Because some OCPs tend to degrade over time and the technical pesticides (i.e., DDT, HCH, chlordane, endosulfan) consist of precise percentage of the different molecules, the ratio between the parent compound and its metabolites can be used as pollution sources indicators. This helps identify whether the concentrations are attributable to fresh or historical use of these substances. The analyzed isomeric ratios showed that, although most OCPs are banned, recent applications of pesticide mixtures still contribute to high soil concentrations in some parts of the study area.

How to cite: Guarino, A., Iannone, A., De Falco, A., and Albanese, S.: Environmental Distribution and Source Analysis of Organochlorine Pesticides in the Soils of the Sarno River Basin, Southern Italy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18593, https://doi.org/10.5194/egusphere-egu25-18593, 2025.

EGU25-20237 | Posters on site | GI5.5

An easy way to build database and analyze data using OnePeterology 

Yi Ding, Tao Wang, Ying Tong, and chaoyang wang

       The 21st century is the era of big data, where scientific research under the new paradigm of data and model-driven knowledge discovery has become the new trend in the scientific field. Under the framework of the international  science project "Deep-time Digital Earth" (DDE), the research team led by Dr. Wang Tao has constructed the OnePetrology database for magmatic rocks. This database adopts a three-in-one approach of "data + mapping + research," based on the magmatic rock knowledge system, with samples as the core,  with self-developed tools to build a magmatic rock database system that integrates big data aggregation and mapping analysis functions.

      The OnePetrology database system includes backend services (cloud), a website (Web), and a scientific research work platform (desktop). The data mainly comes from publicly published literature, tests conducted by the research team, laboratory test data, etc. The data types include basic information on magmatic rock rock types, occurrences, spatial locations, as well as geochronology, geochemistry, (Sr-Nd-Hf-Pb-O) isotopes, and non-traditional (or emerging) isotope data, involving global important orogenic belts, cratons, and some oceans (ocean drilling data).

    The database has preliminarily completed the framework construction and has incorporated a portion of the data, initially forming methods and processes for data aggregation. Currently, there are two ways to contribute data: first, volunteers enter data in the data "data submission portal" set up for this purpose.  The database system has currently built 22 thematic databases and welcomes more disciplinary experts to come to the magmatic rock database to build their own thematic databases.

      The core idea of the database's functionality is to combine big data and software tools for scientific research and exploration. Taking the website as an example, it provides data filtering tools and mapping analysis tools. Data filtering tools include spatial filtering and attribute filtering: spatial filtering can pull cross-sections (set radius), rectangles, custom polygons, global tectonic units, global cratons, China and neighboring areas' main tectonic units, and other search methods, while attribute filtering can set search conditions, value ranges, and fuzzy queries for all fields. Spatial filtering and attribute queries can be used separately or in combination, with query results displayed in table form, spatial distribution maps, and mapping functions. The mapping functions currently built in the database include TAS, Pearce, SiO2-K2O, ACNK-CNK, 2D Density, Heatmap, Profile, etc., each supporting secondary filtering and grouping, facilitating users to quickly discover data patterns.  Currently, online analysis can provide processing capabilities for about 20,000 samples (assuming average desktop computing capabilities). If you need to process larger data volumes, please download the desktop software from the homepage of the website (https://dde.igeodata.org).

     In summary, the DDE OnePetrology magmatic rock database has preliminarily constructed the capabilities for magmatic rock data aggregation and mapping analysis, with other planned functions being built step by step. We warmly welcome more interested experts to participate in the construction and use of the magmatic rock database and to offer your valuable suggestions.

How to cite: Ding, Y., Wang, T., Tong, Y., and wang, C.: An easy way to build database and analyze data using OnePeterology, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20237, https://doi.org/10.5194/egusphere-egu25-20237, 2025.

EGU25-206 | ECS | Orals | EMRP2.2

A Convolutional Neural Network-Based Estimation of Depth to the Bottom of Magnetic Sources from Aeromagnetic Data and Its Applications in Southern Peninsular India 

Arka Roy, Korimilli Naga Durga Prasad, Rajat Kumar Sharma, Dommeti Vijayakumar, and Rajesh Kumar

The magnetic field from Earth's crust helps us understand its thermal structure by finding the depth to the bottom of magnetic sources, an essential indicator of the crustal thermal properties. This study aims to estimate the depth to the bottom of magnetic sources precisely using the magnetic field. Traditional methods, like the spectral peak and centroid techniques, are commonly used to estimate the depth to the bottom of magnetic sources. However, these methods typically require prior knowledge about the magnetization source, derived from empirical relationships of wave-vectors in the spectral domain, which is challenging to obtain over large regions. We devised an innovative deep-learning approach utilizing a convolutional neural network to directly estimate the depth to the bottom of the magnetic sources, eliminating the need for prior knowledge of the fractal magnetization source. Synthetic fractal magnetizations were constructed to train the model, and the performance of the convolutional neural network was compared to the modified centroid approach. Our convolutional neural network methodology was confirmed by utilizing a diverse range of realistic synthetic fractal magnetization, incorporating various window widths and depths to the bottom of the magnetization source. The model is applied to the high-resolution aeromagnetic data of the southern Indian shield to understand the crustal-scale thermal structure.

How to cite: Roy, A., Naga Durga Prasad, K., Sharma, R. K., Vijayakumar, D., and Kumar, R.: A Convolutional Neural Network-Based Estimation of Depth to the Bottom of Magnetic Sources from Aeromagnetic Data and Its Applications in Southern Peninsular India, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-206, https://doi.org/10.5194/egusphere-egu25-206, 2025.

EGU25-455 | ECS | Orals | EMRP2.2

Using a dual-layer gradient-boosted equivalent sources method to grid large magnetic datasets. 

India Uppal, Leonardo Uieda, Vanderlei C Oliveira Jr, and Richard Holme

Towards the construction of a new magnetic map of Antarctica, we investigate the use of gradient-boosted equivalent sources to model data from aeromagnetic surveys. Airborne surveys have larger spacing between adjacent lines compared with along-line spacing. By using the equivalent source technique, gravity and magnetic data can be interpolated onto a regular grid at constant height. This method is particularly useful to prepare the data for further use, such as modelling crustal structures and geological interpretation. The equivalent source technique uses a finite layer of sources to generate the same field as the observed data. These sources are then used to predict the field in unobserved locations. However, estimating the source coefficients that best fit the observed data is computationally demanding. To overcome this problem, the source coefficients are estimated in overlapping windows and carried out iteratively, similar to the gradient boosting method used in machine learning. At each iteration, the sources are fit to the field residuals from the previous iteration. Here we apply the gradient-boosted equivalent sources method to interpolate total-field anomaly observations and convert them to the norm of the anomalous field. We use two layers of equivalent sources at different depths to fit both the regional field and the field due to the shallower sources. We demonstrate using synthetic surveys and an Antarctic magnetic dataset that our dual-layer gradient-boosted equivalent sources are able to produce grids of both the total-field anomaly and the norm of the anomalous field accurately and with a low computational cost.

How to cite: Uppal, I., Uieda, L., Oliveira Jr, V. C., and Holme, R.: Using a dual-layer gradient-boosted equivalent sources method to grid large magnetic datasets., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-455, https://doi.org/10.5194/egusphere-egu25-455, 2025.

EGU25-1139 | ECS | Orals | EMRP2.2

A new numerical tool for the 3D forward modeling of potential field geophysical data in the presence of rugged topography using a numerical integration scheme 

Lahcene Bellounis, Claire Bouligand, Romain Brossier, Ludovic Métivier, and Stéphane Garambois

Potential field geophysical data are frequently used to image geological features in volcanic systems/areas (faults, lithological contacts, alteration zones, geothermal systems, magmatic reservoirs). However, although crucial, it can prove challenging to accurately simulate data in such regions due to the major influence of strong topographic variations. To accurately account for topography with reasonable computational cost, we develop a numerical tool for the modeling and inversion of these data. The method consists of a numerical integration scheme of the integral equations predicting gravity and magnetic data on deformable hexahedral elements. The integrals are evaluated using high-order Gaussian quadrature. Physical properties of the subsurface are defined on discrete grid points, allowing to model discontinuities in the parameters not only at the surface, but also along surfaces within the models, enabling to represent faults, lithological contacts or cavities. Our method uses non-conformal meshes with automatic local refinements in regions with rapidly varying surface topography and in the vicinity of measurement points. In particular, we have developed a local and self-adaptive iterative refinement scheme based on a local convergence criterion of the numerical integration, allowing to reduce the effect of solution singularities close to observation points. The accuracy of our method is tested by comparing our model predictions with results obtained from the tomofast code (https://doi.org/10.5194/gmd-17-2325-2024) using a fine reference discretization of the topography with rectangular prisms. These tests were performed for the modeling of the gravity and magnetic effects of topography over the geothermal system of Krafla, Iceland for the case of ground-based and airborne data. Our modeling tool will ultimately be used for the independent or joint inversion of potential field data to make use of their different sensitivities in terms of physical parameters and also lateral and depth resolutions.

How to cite: Bellounis, L., Bouligand, C., Brossier, R., Métivier, L., and Garambois, S.: A new numerical tool for the 3D forward modeling of potential field geophysical data in the presence of rugged topography using a numerical integration scheme, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1139, https://doi.org/10.5194/egusphere-egu25-1139, 2025.

EGU25-2553 | ECS | Posters on site | EMRP2.2

Contribution of the Combined Analysis of Gravity and Seismic Data in the Study of the Main Hydrogeological Prospects of the Essaouira Basin (Morocco) 

Anas Zbiri, Azzouz Kchikach, Mohammed Jaffal, Mourad Guernouche, Anas Charbaoui, and Guezal Jaouad

This study aims to analyze the deep structure and depression of the thick sedimentary layers to better understand the
geometry and hydrogeology of the aquifers in the Essaouira basin which have been processed through various filters and
transformations. The residual map provides valuable information on density variation, the observed anomalies in the study
area interpreted in term of the topography of the basement, the present of salt deposit and the thickness variation of the
sedimentary series. The seismic reflection profiles covering a limited area in the central-western part of the basin confirm the
gravimetry results and shows that the basin's structure is characterized by a series of anticlines and synclines., resulting from
the combined influences of Atlas tectonics and diapirism. As a result, the shallow aquifer system is broken up into blocks
lifted and collapsed by faults. The result is discontinuous groundwater flow and variable hydrodynamic distribution.
Based on the gravity data processing the principal deep parts of the basin were delineated, including their probable
interconnections-oriented N-S and NNE-SSW. As well, major density contacts (faults) were derived from the enhanced total
horizontal gravity gradient. Their prevailing direction in the central and northern parts of the basin is also N-S and NNE-
SSW; however, it is rather E-W in the southern side. Not all these gravity-based structural-tectonic features match with
geologically mapped faults of NE-SW and NNW-SSE orientation.
The compiled data allowed us to create a structural map that reveals a compartmentalized aquifer system with clearly defined
sub-basins. Additionally, the faults within the Essaouira basin have been precisely mapped. Their predominantly NNE-SSW
orientation suggests a connection to the Triassic rifting of the Atlantic Ocean. It also reveals that the Essaouira basin was
structured in the Triassic and Jurassic periods by a series of deep faults trending in three main directions: NNE-SSW, N-S and
E-W. These results will be invaluable for future oil exploration and hydrogeological research.

How to cite: Zbiri, A., Kchikach, A., Jaffal, M., Guernouche, M., Charbaoui, A., and Jaouad, G.: Contribution of the Combined Analysis of Gravity and Seismic Data in the Study of the Main Hydrogeological Prospects of the Essaouira Basin (Morocco), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2553, https://doi.org/10.5194/egusphere-egu25-2553, 2025.

EGU25-2997 | ECS | Orals | EMRP2.2

Deep learning-based approach to Levelling Airborne Magnetic Data 

Santosh Sanjeev, Meixia Geng, Jiajia Sun, Sultan Abughazal, Qingjie Yang, and Felix Vega

Airborne magnetic surveys provide valuable insights into subsurface structures but often suffer from levelling errors due to inconsistencies between flight lines. These errors, such as striping patterns caused by sensor variations and magnetic field fluctuations, can obscure anomalies and distort interpretations. Traditional corrections like tie-line or micro levelling address these issues but rely on time and frequency domain analyses, making the process labor-intensive, costly, and reliant on expert intervention. Automating and enhancing these workflows is crucial for efficient and accurate levelling across large-scale airborne magnetic datasets. In this work, we propose a deep learning framework for levelling airborne magnetic data by leveraging a U-Net-based architecture. The model is trained in a supervised manner. We use a combination of perceptual loss and mean squared error (MSE) loss to capture fine-grained details while maintaining global consistency in the levelled data. Once trained, the proposed method demonstrates computational efficiency during inference, enabling automatic and robust levelling corrections for large datasets without requiring manual intervention or additional tie-line constraints. The model's performance was evaluated on an independent survey data from the Geological Survey of Brazil database, as well as on an out-of-distribution (OOD) dataset consisting of magnetic field data acquired by Geotech Limited, demonstrating its generalizability and robustness. Our approach demonstrates performance on par with traditional levelling methods, as validated by both quantitative and qualitative metrics, while introducing significant advantages in efficiency and automation. This deep learning-based solution simplifies the levelling process and provides a scalable, adaptive framework designed to meet the demands of modern geophysical surveys.

How to cite: Sanjeev, S., Geng, M., Sun, J., Abughazal, S., Yang, Q., and Vega, F.: Deep learning-based approach to Levelling Airborne Magnetic Data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2997, https://doi.org/10.5194/egusphere-egu25-2997, 2025.

EGU25-3292 | Posters on site | EMRP2.2

Advancements in 3D Potential Field Modeling: Enhancing Lithospheric Insights with IGMAS+ 

Hans-Jürgen Götze, Denis Anikiev, Christian Plonka, Sabine Schmidt, and Magdalena Scheck-Wenderoth

The continuous advancement of geophysical modeling tools has been pivotal in elucidating the complexities of Earth's lithospheric structures. The latest developments in the software package IGMAS+  have introduced innovative techniques for 3D and 4D gravity and magnetic field modeling, combining interactive user control with cutting-edge optimization algorithms. Among these advancements are the integration of space-warping concepts and the Covariance Matrix Adaptation Evolution Strategy (CMA-ES), which provide enhanced precision in inversion processes while preserving model topology. These methods enable the resolution of previously challenging geological scenarios, such as salt dome geometries and rift basin formations. Case studies illustrate the impact of these developments: the Liguro-Provençal Basin's evolution was revisited using gravity field analysis to assess its rifted nature, while applications in the North German Basin demonstrated the effectiveness of the space-warping technique in refining salt dome structures. These examples highlight the added value of such versatility in addressing regional and global geological challenges through multi-disciplinary modeling approaches. By merging forward modeling and interactive inversion with novel numerical methods, the new version of the software provides a robust tool for geoscientists aiming to integrate diverse datasets into comprehensive models. This work underscores the importance of user-driven innovations in geophysical software, pushing the boundaries of how subsurface structures are explored and understood.

How to cite: Götze, H.-J., Anikiev, D., Plonka, C., Schmidt, S., and Scheck-Wenderoth, M.: Advancements in 3D Potential Field Modeling: Enhancing Lithospheric Insights with IGMAS+, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3292, https://doi.org/10.5194/egusphere-egu25-3292, 2025.

EGU25-6049 | ECS | Orals | EMRP2.2

High-resolution aeromagnetic survey over the Tajogaite Volcano, La Palma, Canary Islands 

María C. Romero-Toribio, Fátima Martín-Hernández, and Juanjo Ledo

A high-resolution aeromagnetic survey using a drone was conducted in June 2024 over the Tajogaite volcano on La Palma, Canary Islands. This survey aims to characterise thermal anomalies associated with magma intrusion and the related fault system.

The drone was equipped with a fluxgate magnetometer operating at a sampling rate of 200 Hz, with two sensors separated by 1 m. The constant altitude flights covered approximately a 2.5 km x 2.5 km area, with N-S lines spaced 30–60 m apart. The survey also included tie lines for quality control and calibration flights at very high altitude (low magnetic gradient) to account for the effects of drone pitch, roll, and yaw on magnetic measurements.

Data preprocessing included deriving the total magnetic field from its components, cleaning flight tracks, and compensating for drone-related influences using calibration data. A low-pass filter removed high-frequency noise from the drone’s electronics, and data from both sensors were averaged. Data from all flights were merged and interpolated using linear triangulation onto a 20 m grid with Gaussian smoothing. Diurnal corrections were considered unnecessary due to short flight durations and minimal diurnal variations at low latitudes. Magnetic anomalies were calculated by subtracting the median value from the processed magnetic map.

The new magnetic anomaly map provided critical insights into the thermal and structural characteristics of the volcanic system. This study is part of the GEOTHERPAL project, further detailed at http://pc213fis.fis.ucm.es/GEOTHERPAL/index.html.

How to cite: Romero-Toribio, M. C., Martín-Hernández, F., and Ledo, J.: High-resolution aeromagnetic survey over the Tajogaite Volcano, La Palma, Canary Islands, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6049, https://doi.org/10.5194/egusphere-egu25-6049, 2025.

EGU25-7867 | Orals | EMRP2.2

Optimized Gravity-Magnetic Cross-Gradient Joint Inversion for Characterizing Rift-Sag Geological Structures 

Menglong Xu, Yabin Yang, Zhenning Su, Chuhao Feng, Hongwei Wang, and Li Meng

The geological analysis of rift-sag structures is of significant importance for understanding crustal tectonic evolution, resource exploration, and seismic activity. However, due to the non-uniqueness of gravity and magnetic data inversion and differences in resolution, a single geophysical method often fails to comprehensively reveal the structural characteristics of complex geological bodies. In this study, we propose an optimized gravity-magnetic cross-gradient joint inversion method, introducing several improvements to the weight calculation process. The model weighting matrix and structural constraint weighting matrix are normalized to simplify the calculation formulas, unify the magnitude of the two matrices, and narrow the range for selecting the weighting factors of the cross-gradient term. Furthermore, a dynamic adjustment mechanism for the cross-term weighting factor is adopted, allowing adaptive parameter adjustment based on the variation of model errors, data fitting, and inversion results during the inversion process. This dynamic parameter optimization enhances the inversion results and achieves real-time correction of parameter values, avoiding the limitations of fixed parameters and improving the reliability of the inversion.

The proposed method was applied to measured gravity and magnetic profiles in the southern margin of the Sichuan Basin. By integrating planar gravity and magnetic anomaly characteristics with vertical boundary identification techniques, the gravity field, magnetic field, structural features, deep characteristics, and sedimentary features of the rift-sag structure were systematically analyzed. The results provide reliable evidence for delineating the spatial distribution of rift-sag boundaries and the internal geological features, offering robust support for geological research and geophysical interpretations in complex tectonic environments.

Acknowledgments: This research was funded by the National Natural Science Foundation of China [grant numbers: 42104092], Fundamental Research Funds Program of Chinese Academy of Geological Sciences [grant numbers: JKYQN202351].

How to cite: Xu, M., Yang, Y., Su, Z., Feng, C., Wang, H., and Meng, L.: Optimized Gravity-Magnetic Cross-Gradient Joint Inversion for Characterizing Rift-Sag Geological Structures, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7867, https://doi.org/10.5194/egusphere-egu25-7867, 2025.

EGU25-9345 | Posters on site | EMRP2.2

Exploring the Lake Hazar (Elazığ-Turkey) Basin Geometry with Vertical Prismatic Polyhedra 

Nedim Gökhan Aydın and Turgay İşseven

The Lake Hazar pull-apart basin, situated along the East Anatolian Fault System, represents a key tectonic structure within one of Turkey's most active seismic zones. This fault system recently generated two catastrophic M7.0+ earthquakes in February 2023, underscoring the importance of understanding its associated geological features. Gravity modeling offers a powerful tool for exploring such basins, providing insights into subsurface geometry and tectonic processes.

This study employs vertical prismatic polyhedra to model the basin. Conventional modelling methods often require a trade-off between computational efficiency and data resolution, either overloading calculations with unnecessary prisms or losing critical detail with coarse sampling. By integrating Voronoi diagrams into the modeling process, we achieve sensitivity to data sampling frequency while maintaining computational efficiency and preserving accuracy.

Approximately 600 newly collected gravity data points from the Sivrice and Gezin provinces were used to construct the two-layer models. Forward modeling with a constant density contrast yielded basin geometries to a maximum depth of 350 meters, achieving root-mean-square errors below 0.1 mGals. Beyond refining the 3D basin structure, this method allowed us to estimate excess mass within different sections, providing additional constraints on sedimentary characteristics and tectonic activity in the region.

Comparison with our previous 2D-to-quasi-3D Talwani models revealed consistent results, including similar sediment thickness variations. However, the vertical prismatic polyhedra method demonstrated superior adaptability to irregularly spaced data and greater computational efficiency, making it especially suitable for complex tectonic environments like the Lake Hazar region. The integration of computationally efficient methods highlights the potential for future applications in similar tectonic settings, advancing our ability to investigate fault-controlled basins in active seismic regions.

How to cite: Aydın, N. G. and İşseven, T.: Exploring the Lake Hazar (Elazığ-Turkey) Basin Geometry with Vertical Prismatic Polyhedra, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9345, https://doi.org/10.5194/egusphere-egu25-9345, 2025.

EGU25-9602 | ECS | Posters on site | EMRP2.2

Imaging the shallow magmatic system of the Xiangshan volcanic basin by the 3-D joint inversion of potential field data 

Min Feng, Juzhi Deng, Hui Chen, Hui Yu, and Xiao Chen

The underlying magmatic system in the Xiangshan volcanic basin is crucial in controlling the origin and migration of ore-forming fluids and driving uranium element transport. However, its shallow structure still lacks high-resolution imaging constraints. Gravity and magnetic data are combined in a three-dimensional joint inversion to obtain structurally similar density and magnetic susceptibility models of the Xiangshan shallow magmatic system. As imaged by the obtained model, a steep tubular anomaly characterized by low density and high magnetic susceptibility beneath the main peak of Xiangshan, interpreted to be a volcanic conduit associated with the porphyroclastic lava. A tubular high-magnetic susceptibility anomaly that located approximately 3 km west of the Xiangshan main peak is also imaged, is presumed to be a rhyodacite volcanic conduit. Both of them converge at depth and exhibit a hereditary relationship. In addition, the east-west oriented low-density anomaly is likely a reflection of the depression zone in the metamorphic basement. It is speculated that the imaged regional structural framework could control the emplacement of shallow magmatic system. We argue that the deep magma intrudes along the basement fault zone and ascends through its derived secondary fractures, providing material and heat sources for shallow hydrothermal circulation.

This work was funded by the National Natural Science Foundation of China (grants 42130811, 42304090 and 42374097) and by Jiangxi Provincial Natural Science Foundation (20242BAB20143).

How to cite: Feng, M., Deng, J., Chen, H., Yu, H., and Chen, X.: Imaging the shallow magmatic system of the Xiangshan volcanic basin by the 3-D joint inversion of potential field data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9602, https://doi.org/10.5194/egusphere-egu25-9602, 2025.

EGU25-12062 | Posters on site | EMRP2.2

Towards More Reliable Surface Geometry Inversion Methods for Mineral Exploration 

Saeed Vatankhah and Peter Lelievre

Most large and easily accessible mineral deposits have been found and exploited. To continue to supply critical mineral resources central to global industries, mineral exploration must move to deposits that are deeper or smaller, and therefore are more challenging to identify and characterize using geophysical methods. To provide reliable imaging results for these challenging scenarios, new inversion techniques are required that can reduce the non-uniqueness of the inverse problem through tight integration of geophysical and geological data.

For this purpose, we are studying surface-geometry inversion (SGI) methods, which parameterize the Earth in terms of surfaces representing interfaces between different rock units. This parameterization is more consistent with geologists' understandings of the Earth, and has high potential to allow the tight integration of geophysical and geological information that we seek. Our SGI approach effectively takes some initial surface-based model, for example a geological model, and alters the position of the surfaces to improve the fit to the geophysical data. Using geophysical inversion to determine the geometry of subsurface targets has a long-established history, tracing back to the early days of geophysical interpretation. These methods continue to gain considerable attention because of the growing demand for more precise and interpretable visual representations of subsurface bodies.

Recently, SGI methods are becoming increasingly common and have been applied to many varied imaging scenarios. However, little work has thoroughly assessed the reliability of these methods. It is important to know whether the solutions obtained from SGI are unique and stable and, if they are not, how to add regularization or constraints to make them so. Without a well-posed problem, any interpretations of the subsurface based on those solutions, and any exploration decisions based on those interpretations, are unreliable. Assessing the numerical characteristics of SGI problems is challenging because they overwhelmingly use global heuristic optimization methods and stochastic sampling in their solution, they are severely nonlinear, and they lack explicit matrix operators and derivatives. A critical aspect is understanding when regularization/stabilization should be incorporated into the SGI optimization problem to create a well-posed problem. In this work, we make headway towards a better understanding of these important issues in the specific context of inverting potential field data for mineral exploration scenarios.

How to cite: Vatankhah, S. and Lelievre, P.: Towards More Reliable Surface Geometry Inversion Methods for Mineral Exploration, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12062, https://doi.org/10.5194/egusphere-egu25-12062, 2025.

EGU25-12869 | Orals | EMRP2.2

Magnetic Anomalies: Anywhere and Anytime – Accurate Information for Use in Alternative Navigation 

Rick Saltus, Arnaud Chulliat, and Annette Balmes

Alternative navigation (AltNav) includes development of magnetic navigation (MagNav) using the Earth’s magnetic field as a reference. Current implementation requires highly accurate estimates of the full expected magnetic field along the predicted travel path. This is a challenging problem.

This presentation focuses on delivery of trustable estimates of the crustal magnetic anomaly as a component of the full field. In many operational situations (depending on altitude and speed), the variations of the crustal magnetic field represent the primary signal for use in MagNav.

One key challenge is the integration of original survey data into a comprehensive grid/model with accompanying estimation of the anomaly uncertainty. The required resolution and accuracy of this information will vary depending on navigational operation, but current MagNav implementations are dependent on highly accurate anomaly estimation. To meet this requirement, it is important to assess and optimize: (1) the quality and sampling of the original survey data; (2) the methods used to interpolate the survey data into a regular grid; and (3) the upward (or downward) continuation of the data (both for anomaly and directional gradient) to the required navigational position.

We report on methods developed for these 3 requirements using (1) FFT-based power spectrum analysis of initial survey sampling, (2) a new method for magnetic grid cell uncertainty estimation, and (3) experimentation with generalized equivalent source techniques for on-the-fly calculation of anomaly and directional gradient at selected locations.

How to cite: Saltus, R., Chulliat, A., and Balmes, A.: Magnetic Anomalies: Anywhere and Anytime – Accurate Information for Use in Alternative Navigation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12869, https://doi.org/10.5194/egusphere-egu25-12869, 2025.

Existing global-scale models of the Earth’s lithospheric magnetic field are composed of short wavelength information (< 100 km) from near-surface survey data and long wavelength information (> 300 km) from satellite data. In oceanic areas, compilations of ship trackline data provide the near-surface measurements used to construct gridded maps of the crustal magnetic anomaly field. Although these maps have been used widely for tectonic and geodynamic studies, advanced applications, including complex inversions, machine learning, and the use of magnetics for alternative (to GPS) navigation, require renewed attention as to how gridded maps are made. Data selection, including detection of anomalous tracklines, knowledge of the sampling and power spectra of the potential field, quantification of uncertainty and an accurate representation of the gradients in the estimated field all represent areas of interest for advanced applications.

We help address the problem of magnetic map-making for advanced applications by developing a means of quantitative comparison of magnetic data which is applied to each length scale of the underlying magnetic measurements and interpolated grids as a function of potential field frequency (spatial wavelength). Coherence analysis provides a technique to make a wavelength-dependent quantitative comparison, which can be used for data selection as well as to measure length-scale dependent attributes, errors, and uncertainties. Coherence can help to assess if individual tracklines are consistent with the overall dataset and help to determine if anomalous tracklines should be included in a final map product. Applied in this way, coherence could help automate or semi-automate the task of trackline selection. Coherence can be used to evaluate gridded maps made using different procedures for interpolation and continuation, helping to identify optimal map-making methods.

The coherence method also can be used to validate map quality in specific locations by comparing single trackline survey data to the reference map in the trackline direction using one-dimensional coherence, evaluating map quality and errors over several length scales. An understanding of the uncertainty at different length scales provides important information for the development and tuning of navigation algorithms and can provide an analytical framework for understanding different methods of map construction. In areas with high-quality reference maps this type of analysis can help inform scale dependent uncertainty models.

How to cite: Duff, P. and Nielsen, A.: Magnetic map-making for advanced applications: Quantitative comparison of frequency dependent features, errors, and uncertainties in gridded magnetic data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14009, https://doi.org/10.5194/egusphere-egu25-14009, 2025.

EGU25-14485 | ECS | Posters on site | EMRP2.2

High-precision Magnetization Vector Inversion : Application to the Mineral Exploration 

Xiangdong Li and Shuang Liu

  Magnetization vector inversion is essential for obtaining magnetization vector information from subsurface rocks. To obtain focused inversion results that better match the true magnetization distributions, sparse constraints are considered to constrain the objective function. A compact magnetization vector inversion method is proposed that can provide accurate inversion results for magnetic data with significant remanent magnetization. Considering the sparse constraint and the correlation between the three magnetization components with different directions, the L1-norm is modified and introduced into the inversion algorithm to obtain compact results.Furthermore, to reduce the computational cost, a randomized singular value decomposition is used to replace the traditional singular value decomposition and iteratively minimize the proposed objective function. Finally, the proposed method is applied to igneous rocks with strong remanent magnetization in the Haba River area of northwestern China. The distributions, directions of total magnetization and remanent magnetization of the medium-base igneous rocks are revealed by the sparse magnetization vector inversion method, which provides a wealth of information about the concealed deposits in the area.

How to cite: Li, X. and Liu, S.: High-precision Magnetization Vector Inversion : Application to the Mineral Exploration, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14485, https://doi.org/10.5194/egusphere-egu25-14485, 2025.

EGU25-14488 | Posters on site | EMRP2.2

3D Compact Geometry Inversion for Gravity Data 

Baifan Zhang and Shuang Liu

Gravity inversion quantitatively provides a 3D model of density contrasts, significantly enhancing the information extracted from acquired data. However, the inherent non-uniqueness of inversion poses challenges in precisely determining the boundaries of anomalous bodies. We have developed an iterative algorithm of gravity inversion that reconstructs the geometric features of the anomalous bodies by discretizing the 3D interpretation model with vertical and juxtaposed prism cells. These prisms incorporate sheet-like initial models which are typically derived from prior information or imaging results. This study proposed a new parameter, the Thickness Factor (TF), which is determined by the thickness of the prism cells under the assumption of homogeneous anomalous bodies. The TF establishes an approximate linear relationship between the source geometry and gravity anomalies, enabling the reconstruction of the source geometry to be formulated as a linear optimization problem. The approach demonstrates the potential for target inversion in the presence of multiple causative sources in synthetic cases and shows insensitivity to noise signals and reliability in reconstructing the geometry of complex sources. The proposed method is then applied to real data from the Galinge iron ore deposit in Northwest China and the drilling data is used as prior information. The inversion results are consistent with previous drilling interpretations and allow a rough estimation of the volume of the ore bodies.

How to cite: Zhang, B. and Liu, S.: 3D Compact Geometry Inversion for Gravity Data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14488, https://doi.org/10.5194/egusphere-egu25-14488, 2025.

EGU25-15102 | Posters on site | EMRP2.2

A fast inversion method for magnetic components 

Deliang Teng, Linfei Wang, Jinxin Zheng, Guanxin Wang, and Dianjun Xue

Vector geomagnetic survey technique can obtain simultaneously the magnitude and direction information of the geomagnetic field, which can effectively reduce the multiplicity of solutions on the inversion, contribute to the quantitative interpretation of the magnetic body, so as to improves the detection resolution and positioning accuracy of the ore. The development of magnetic component inversion is restricted by factors such as the estimation accuracy of the direction of magnetization, the calculation efficiency of the objective function. According to the analytic solution formula of the magnetic component, three kernel matrices can be constructed to calculate the magnetic components Bx, By, and Bz by using the magnetization intensity, which can not only avoid the prior estimation of the direction of the magnetization, but also the constructed kernel matrix is a blocky toeplitz matrix with the help of the special blocking method of the equivalent geometric architecture. And because of the structureal properties of the blocky toeplitz matrix, the computational of the kernel matrix and magnetization intensity is simplified and the huge storage consumption is reduced.Finally, the regularization method is used to invert the solution. A theoretical model is used to verify the utility and reliability of the method.The result shows that compared with the traditional method, the computational time of the proposed method is reduced greatly, and the inversion results are consistent with the input model.

How to cite: Teng, D., Wang, L., Zheng, J., Wang, G., and Xue, D.: A fast inversion method for magnetic components, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15102, https://doi.org/10.5194/egusphere-egu25-15102, 2025.

EGU25-16540 | ECS | Orals | EMRP2.2

DEXP imaging of potential fields with multi-homogeneity theory 

Luigi Bianco and Maurizio Fedi

One of the most interesting properties of the gravity fields generated by ideal sources (e.g., sphere, dyke, sill and contact)is that they are homogeneous functions of integer degree n, ranging from -2 to 1. It is to say that they satisfy the homogeneity equation in the harmonic region. However, when the source distribution is more complex than that of ideal sources, fields are not homogeneous. When analyzed at different distances, these fields will have different homogeneity degrees which can assume also a fractional and distance-dependent value. This results in the multi-homogeneity law which accounts for n varying at each observation site.

Accordingly, we may introduce the multi-homogeneity theory into the Depth From Extreme Points (DEXP) method. DEXP is an imaging method, which is based on field transformations, not involving any inverse matrix, so being faster and simpler to use. An important role in the scaling of the modelled field is played by the exponent N, the structural index. N is a parameter characterizing the type of source and is directly related to n as N=-n+q with q being the differentiation order of the Newtonian potential.

The proposed DEXP transformation for general sources is based on the multi-homogeneity theory so that the field is scaled by the inhomogeneous exponent N (x,y,z).

DEXP imaging of synthetic and real data demonstrated the ability to interpret complex bodies geometries which are brought by the DEXP method with the multi-homogeneity theory.

How to cite: Bianco, L. and Fedi, M.: DEXP imaging of potential fields with multi-homogeneity theory, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16540, https://doi.org/10.5194/egusphere-egu25-16540, 2025.

EGU25-16657 | ECS | Posters on site | EMRP2.2

Training a CNN network with powerful but simple models 

Ciro Messina, Luigi Bianco, and Maurizio Fedi

       This study wants to show how  a Convolutional Neural Network may be trained by models built on a simple but strong a priori information—in this case, the gravitational field of a fault—can allow a good reconstruction of complex 3D structures. The key innovation is to train the algorithm with elementary source models. These elementary blocks consist of fault models with varying parameters such as dip, density contrast, thickness, and depth to the top. For each anomaly, profiles are extracted from the anomaly map, subdivided into two sub-profiles, and interpreted using the fault-based ML algorithm. This workflow follows the idea that gravimetric anomalies, when analysed along a profile crossing the source, can be seen as composed by the constructive interference of anomalies generated by the edges of the source bodies reducible to faults. The interpreted sections are then interpolated to create a reference 3D model, which yields a strong information, as a reference model, for a final 3D inversion process, which refines the model and yields a good data-misfit.

 To validate the method, we applied it to two different cases: a synthetic diapir-shaped source and a real geological structure, the Caltanissetta basin in Sicily (Italy). In both cases, the method successfully reconstructed the different structures.

How to cite: Messina, C., Bianco, L., and Fedi, M.: Training a CNN network with powerful but simple models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16657, https://doi.org/10.5194/egusphere-egu25-16657, 2025.

EGU25-16898 | Orals | EMRP2.2

FIQUgS Innovations in Quantum Gravity Sensing: Data Processing for an Archeological Case Study 

Daniele Sampietro, Martina Capponi, and Camille Janvier

The FIQUgS project represents a transformative step forward in geophysical research, combining cutting-edge quantum gravity sensing technology with advanced software tools to enhance subsurface exploration. A landmark demonstration of these capabilities occurred in October 2024 in Lisbon, Portugal, during a collaborative archaeological study with the Centro de Arqueologia de Lisboa. This case study aimed to detect and characterize shallow tunnels and cavities from the Roman era beneath Lisbon’s historic center, leveraging the Differential Quantum Gravimeter (DQG) and a suite of sophisticated data processing software.  The work presented here aims to enter into the details of data processing from the preliminary stage of survey planning to the post processing inversion and interpretation of data.

Central to this first real outdoor application of the DQG, was the FIQUgS survey planning tool, which used statistical inference to optimize survey paths and observation point spacing. This tool minimized data acquisition efforts while maximizing the sensitivity of detection capabilities. Post-survey, the collected data underwent extensive processing using FIQUgS-developed algorithms designed to refine gravity anomaly and vertical gravity gradient measurements. The vertical gravity gradient measurements proved particularly advantageous, significantly reducing the impact of distant mass effects and environmental noise, thereby enhancing the clarity of subsurface features.  

An integral part of the data analysis was the automated inversion module, which used the processed measurements to reconstruct the geometry of subsurface structures. The module successfully identified and modeled a Roman-era tunnel with an estimated cross-sectional area of approximately 5 square meters. By integrating additional geophysical data, such as digital terrain models, the inversion tool further improved the accuracy of the subsurface density distribution.  

This case study highlights the practical value of FIQUgS software innovations in real-world applications. The seamless integration of advanced survey planning, data processing, and inversion tools allowed for a comprehensive analysis of complex subsurface conditions. The success of the Lisbon study underscores the potential of quantum gravity sensors and associated software to address long-standing challenges in geophysical research and archaeological exploration. As the FIQUgS project continues to develop, these technologies promise broader applicability in areas such as mineral exploration, groundwater management, and structural monitoring.  

This achievement demonstrates the synergy between hardware and software in advancing geophysical methodologies, paving the way for more efficient and precise subsurface investigations across diverse scientific and industrial domains.

How to cite: Sampietro, D., Capponi, M., and Janvier, C.: FIQUgS Innovations in Quantum Gravity Sensing: Data Processing for an Archeological Case Study, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16898, https://doi.org/10.5194/egusphere-egu25-16898, 2025.

EGU25-17417 | Posters on site | EMRP2.2

Participative gravity-modelling of the Balmuccia peridotite body: progress report 

Ludovic Baron, Matteo Scarponi, Denis Anikiev, Enikő Barbély, Judit Benedek, Hans-Jürgen Götze, Mohammad Ismaiel, Gábor Papp, Sabine Schmidt, Rosaria Tondi, and György Hetényi

The Balmuccia peridotite is a well-known outcrop in the Italian Alps, with a surface extent of ca. 4.4 km. by 0.6 km, including a ca. 1000 m elevation change. It is of particular interest for project DIVE (Drilling the Ivrea-Verbano zonE, ICDP expedition 5071) phase 2 as it is a prime site to continuously sample the crust–mantle transition by drilling, and to test the suitability of a natural peridotite body for serpentinization and hydrogen production.

Current models of the subsurface extent of the Balmuccia peridotite differ significantly, depending not only on the geoscience discipline of investigation, but also on the characteristics of the geophysical imaging campaigns. Therefore, in an effort to reduce the uncertainties regarding the geometry of the Balmuccia peridotite body at depth, we have launched an open, participative gravity-modelling challenge (Hetényi et al. 2024): a new gravity dataset of 151 points is shared with anyone interested, accompanied by a geological map, rock densities of the different lithologies, and a digital elevation model. Interested parties can design various 3D model setups and perform modelling and/or inversion, the results of which can then be compared.

In the past year, several groups have shown interest in modelling the target body, and have undertaken processing steps, corrections, and defined model geometry classes for forward modelling. While the initial concept was to let each group work independently, regular meetings allowed to agree on a few steps beyond what was provided with the data (such as an optimized DEM to be used by all participants), and to discuss individual questions regarding the data and the computations. In this contribution we will present the progress of this initiative, compare existing models or their elements, taking into account other geophysical data beyond gravimetric measurements, and outline the remaining questions. Preliminary conclusions regarding the geometry of the Balmuccia peridotite body are planned to be presented.

How to cite: Baron, L., Scarponi, M., Anikiev, D., Barbély, E., Benedek, J., Götze, H.-J., Ismaiel, M., Papp, G., Schmidt, S., Tondi, R., and Hetényi, G.: Participative gravity-modelling of the Balmuccia peridotite body: progress report, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17417, https://doi.org/10.5194/egusphere-egu25-17417, 2025.

EGU25-19366 | Orals | EMRP2.2

Contrasting geothermal heat flux provinces unveiled beneath Antarctic subglacial lake districts 

Fausto Ferraccioli, Pietro Latorraca, Shi Quan Ooi, Jonathan Ford, Ben Mather, Egidio Armadillo, Joerg Ebbing, Graeme Eagles, Karsten Gohl, Rene Forsberg, Chris Green, Javier Fullea, and Massimo Verdoya

Antarctic geothermal heat flux (GHF) is poorly known restricting our ability to assess its influence on subglacial hydrology and ice sheet dynamics. Within the 4D Antarctica and the 3D Earth ESA projects, a new Antarctic aeromagnetic anomaly compilation, conformed at long wavelengths with SWARM satellite magnetic data was complied. All the datasets were levelled, microlevelled and stitched together. We also differentially continued all survey data to 4 km and re-gridded the compilation onto a 4 km grid mesh.

Our new aeromagnetic anomaly compilation enables us to re-assess Antarctic geothermal heat flux (GHF) heterogeneity, a critical basal boundary condition that influences Antarctic ice sheet flow and subglacial melting and hydrology. To estimate GHF we applied Curie Depth Point (CDP) estimation using the centroid, modified centroid and fractal/defractal approaches. We compared our CDP results with independent constraints on crustal and lithosphere thickness derived from seismological, airborne gravity and satellite gravity modelling and effective elastic thickness estimates. We also considered empirical estimates of GHF derived from seismology and recent models of intracrustal heat production from gravity inversion to assess additional uncertainties associated with CDP to GHF conversion. We performed both automated continental scale estimates and nested manual analysis of CDP and GHF with a specific focus on different Antarctic subglacial lake districts.

We found elevated GHF in the West Antarctic Rift System (WARS) beneath the rapidly changing Thwaites (THW) and Pine Island sectors of the West Antarctic Ice Sheet (WAIS) and along the edge of the Marie Byrd Land block. Focussed estimates of GHF were performed over the cascading active lakes beneath THW to provide new constraints for hydrological modelling in this critical sector of the WAIS. We image a large degree of heterogeneity in thermal basal boundary conditions beneath the active subglacial lake districts that underlie the ice streams flowing into the Ross Sea Embayment, which we relate to hitherto poorly known tectono-magmatic segmentation of the WARS.

In East Antarctica, elevated GHF is associated with some of the active lakes underlying the Byrd glacier catchment, but relatively lower GHF values are typical of both the active and static lakes of the northern Wilkes Subglacial Basin (WSB). This suggests limited upper crustal extension beneath this enigmatic subglacial basin compared to major Mesozoic to Cenozoic extension in the WARS. These findings agree with current seismological evidence for well-preserved fast and cold craton margin lithosphere beneath most of the WSB.

We image relatively elevated GHF beneath the Dome C and Dome A subglacial lake districts. This may be caused by cryptic but large-scale provinces of high heat producing Precambrian basement or could reflect major intraplate reactivation of Precambrian fault systems. Elevated GHF is also imaged in Dronning Maud Land and stretching from Enderby Land to Princess Elizabeth Land. We propose that this could reflect Cambrian age lithosphere thinning due to orogenic collapse processes that affected major and yet still cryptic paths of Gondwana-forming orogenic belts fringing East Antarctica. Additionally, Jurassic to Cretaceous thinning was likely superimposed and associated with passive margin formation during Gondwana break-up. 

How to cite: Ferraccioli, F., Latorraca, P., Ooi, S. Q., Ford, J., Mather, B., Armadillo, E., Ebbing, J., Eagles, G., Gohl, K., Forsberg, R., Green, C., Fullea, J., and Verdoya, M.: Contrasting geothermal heat flux provinces unveiled beneath Antarctic subglacial lake districts, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19366, https://doi.org/10.5194/egusphere-egu25-19366, 2025.

EGU25-19768 | Posters on site | EMRP2.2

Assessing the CO2 stored mass at the Sleipner storage site from time lapse gravity data 

Maurizio Milano, Luigi Bianco, and Maurizio Fedi

This study shows that multiscale imaging methods applied to time-lapse gravity data can be effective to estimate the subsurface stored mass of CO₂. Differently from previous studies based on simplified plume shapes, we show that a multiscale analysis of gravity data is particularly useful to properly estimate the excess mass from gravity anomalies associated with complex plume geometries and characterized by multi-homogeneity properties. With a multiscale approach, in fact, we can exploit the scaling behavior of the potential fields and assess the variation in the degree of homogeneity and, consequently, the estimation of the structural index of the source. 

The simulated gravity dataset and the estimated homogeneity degree values at different altitudes showed that, as the distance from the source increases, the gravity field associated with the CO2 plume becomes progressively smooth and can be approximated as homogeneous. Moreover, the multiscale analysis effectively reduces the noise effect, that is particularly advantageous for CO2 storage monitoring, where low signal-to-noise ratios are expected. The excess mass inferred using our approach results closely equal to the true value with accuracy higher than 99%. Our multiscale analysis was also successfully applied to the real time-lapse gravity dataset acquired at the Sleipner site.

This study presents a useful approach for developing new monitoring strategies for CCS purposes. Time-lapse gravity surveying has again proven to be an effective tool for inferring key reservoir properties, complementing seismic monitoring techniques.

How to cite: Milano, M., Bianco, L., and Fedi, M.: Assessing the CO2 stored mass at the Sleipner storage site from time lapse gravity data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19768, https://doi.org/10.5194/egusphere-egu25-19768, 2025.

EGU25-20682 | ECS | Posters on site | EMRP2.2

Training Super-Resolution deep learning algorithms for high resolution aeromagnetic maps generation from low resolution aeromagnetic maps. 

Eric Penda biondokin, Mojtaba Bavandsavadkoohi, shiva Tirdad, and Erwan Gloaguen

The province of Quebec (Canada) is regarded as the principal mining Province of Canada due to its substantial exploitable reserves and the significant contribution of its mineral production to the national GDP. Nevertheless, Vast areas, such as northern Quebec, remain insufficiently covered in terms of geoscientific data, limiting the understanding of their mineral exploration potential.

Aeromagnetic data are widely employed for large-scale reconnaissance to map geological structures and guide geologists in identifying exploration targets or defining new prospects. However, the only data that covers the entire area are low-resolution aeromagnetic data, with high-resolution datasets being sporadically available. This low resolution restricts the interpretability of regional data, as certain geological structures remain hidden by coarse sampling intervals. To enhance geological mapping, it is imperative to improve the resolution of aeromagnetic data to reveal structures such as faults, lineaments, and lithological boundaries that are otherwise undetectable in low-resolution geophysical signatures. While acquiring high-resolution data is an ideal solution, the high costs and vast territorial coverage required render this approach challenging in the short term. As an alternative, the advent of artificial intelligence (AI), particularly deep learning, offers promising avenues for exploration. In this study, we adapted and retrained 4 super-resolution deep learning algorithms to generate high resolution aeromagnetic maps from low resolution ones. To avoid bias due to spatial correlation, we split the data sets into a training set covering the southern part of Québec and validation being the Northern part. Each of the AI codes were trained on the same datasets leading to optimal hyperparameters for each algorithm. The AI-generated results for all the 4 algorithms successfully reconstruct high-resolution regional aeromagnetic maps in the training sets compared to measured high resolution data providing reliable high resolution maps for geological mapping. Finally, we generated four high resolution aeromagnetic maps for entire Province including the northern part. This innovative approach holds the potential to revolutionize geophysical exploration, facilitating the discovery of untapped natural resources in underexplored areas

How to cite: Penda biondokin, E., Bavandsavadkoohi, M., Tirdad, S., and Gloaguen, E.: Training Super-Resolution deep learning algorithms for high resolution aeromagnetic maps generation from low resolution aeromagnetic maps., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20682, https://doi.org/10.5194/egusphere-egu25-20682, 2025.

EGU25-518 | ECS | Orals | PS7.5

Evidence for very recent tectonic activity in southern Tharsis 

Bartosz Pieterek, Petr Brož, Ernst Hauber, and Oguzcan Karagoz

The formation of Tharsis affected nearly the entire western hemisphere of Mars and had a profound effect on Martian geodynamics. Tharsis-related lithospheric deformation created a variety of tectonic structures that record past stress fields, some of which may still be active today. However, evidence for very recent endogenic activity (<1 Ma) in Tharsis remains limited even after the seismic measurements by the NASA InSight mission. Very few morphologically pristine tectonic structures have been discovered in remote sensing data, limiting our understanding of the current endogenic activity in Tharsis.

Building on our previous research in the southeastern Tharsis region, we focus on the Claritas Fossae region. This area displays several cross-cutting fracture and fault sets, recording a complex history of multiple volcano-tectonic events. Using High Resolution Imaging Science Experiment (HiRISE) images and stereo image-derived Digital Elevation Models (DEMs), we identified uphill-facing scarps on the west-facing Claritas Rupes scarp, which bounds a major N-S-trending extensional structure, informally called the Thaumasia Graben. The two-kilometer-high steep slopes of Claritas Rupes experience intense mass wasting, producing rockfalls (boulders) that accumulate against these uphill-facing scarps. Despite the high boulder fall rates, which over time could fill the accommodation space created by the uphill-facing scarps and mask them, small of these scarps retain a pristine topography. These observations suggest a very young age (<1 Ma) for these scarps. We interpret these scarps as surface expressions of normal faulting linked to Deep-seated Gravitational Slope Deformations (DGSDs), likely caused by seismic activity tied to reactivation of the Claritas Rupes fault associated with Thaumasia Graben subsidence. This indicates neotectonic activity in the region, which is potentially still ongoing.

To better constrain the tectonic processes and the mechanism of the very recent small-scale faulting at the Claritas Rupes scarp, our current structural mapping aims at deciphering the orientations and the spatiotemporal relationships of these scarps. Our approach involves obtaining dip angles through a planar fitting method and quantifying shortening along mapped scarp features. This forms the basis for determining effective stress distribution under isotropic stress conditions with plane strain assumptions, offering insights into the youngest stages of the tectonic evolution of this region. Our satellite image-based morphological investigations focusing on fresh-looking scarps show great advances in tectonic feature mapping, offering valuable insights into inaccessible subsurface endogenic processes in southeastern Tharsis.

How to cite: Pieterek, B., Brož, P., Hauber, E., and Karagoz, O.: Evidence for very recent tectonic activity in southern Tharsis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-518, https://doi.org/10.5194/egusphere-egu25-518, 2025.

EGU25-2216 | ECS | Orals | PS7.5

3D Gaussian Splatting for Detailed Reconstruction of Planetary Surfaces from Orbiter Images 

Zhaojin Li, Bo Wu, and Shihan Chen

Three-dimensional (3D) mapping of planetary surfaces is critical for exploration missions and scientific research (Gwinner et al., 2016). Previous research mainly focused on employing rigorous techniques such as photogrammetry and photoclinometry to generate topographic products such as digital elevation models (DEMs). While the integration of these two techniques can yield detailed and precise topographic data, photoclinometric algorithms are heavily dependent on radiometric data and surface reflectance behaviors (Chen, Hu, et al., 2024; Liu and Wu, 2023), which limits their use in different circumstances. This paper undertakes a new endeavor to explore the potential of the emerging 3D Gaussian splatting techniques for a detailed reconstruction of planetary surfaces from orbiter images.

Gaussian Splatting has demonstrated outstanding performance in 3D applications for close-range scenes and has recently attracted significant attention. The primary challenge in utilizing 3D Gaussian Splatting for the reconstruction of planetary surfaces from orbiter images lies in the complexity of the planetary push-broom camera models. The sophisticated camera model and projection algorithm complicate this optimization approach. To address this, a two-step approach is proposed to transform the planetary push-broom images into frame-like images. First, photogrammetry is applied to push-broom images to extract precise 3D topography, which is then textured using the corresponding textures from the orthoimages. From the textured 3D landscape, frame images are rendered with careful consideration of overlapping and lighting conditions to better support 3D reconstruction tasks. For surface reconstruction, the 2D Gaussian splatting method (Chen., Li., et al., 2024) is selected and implemented in a coarse-to-fine manner, incorporating a smoothness loss to ensure its suitability for textureless planetary surfaces. In addition to utilizing information from the images, the algorithm also takes into account the camera geometry derived from the previous two steps for improved 3D surface reconstruction.

Experiment analysis is conducted using HiRISE images covering the Jezero crater on Mars. The photogrammetric DEM is generated at a resolution of 1 meter per pixel, and the original images are rectified and mosaicked at their native resolution of 0.25 meters per pixel. A total of 421 frame images are rendered, ensuring high overlapping (e.g., one point appears in eight rendered images) coverages. Compared to the photogrammetric DEM, the DEM generated by 3D Gaussian splatting reveals more subtle topographic details and maintains geometric accuracy.

 

Reference

Chen, D., Li, H., Ye, W., Wang, Y., et al., 2024. PGSR: Planar-based Gaussian Splatting for Efficient and High-Fidelity Surface Reconstruction. arXiv preprint arXiv:2406.06521.

Chen, H., Hu, X., Willner, K., Ye, Z., et al., 2024. Neural implicit shape modeling for small planetary bodies from multi-view images using a mask-based classification sampling strategy. ISPRS Journal of Photogrammetry and Remote Sensing 212, pp. 122-145.

Liu, W.C., Wu, B., 2023. Atmosphere-aware photoclinometry for pixel-wise 3D topographic mapping of Mars. ISPRS Journal of Photogrammetry and Remote Sensing 204, pp. 237-256.

Gwinner, K., Jaumann, R., Hauber, E., Hoffmann, et al., 2016. The High Resolution Stereo Camera (HRSC) of Mars Express and its approach to science analysis and mapping for Mars and its satellites. Planetary and Space Science 126, pp. 93-138.

How to cite: Li, Z., Wu, B., and Chen, S.: 3D Gaussian Splatting for Detailed Reconstruction of Planetary Surfaces from Orbiter Images, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2216, https://doi.org/10.5194/egusphere-egu25-2216, 2025.

EGU25-3321 | ECS | Posters on site | PS7.5

High-resolution Topographic Modeling for the Lunar South Pole Region Using NAC and ShadowCam Images 

Hao Chen, Philipp Gläser, Konrad Willner, Qian Huang, Xiaohuan Xie, and Jürgen Oberst

Illumination conditions in the lunar polar areas are highly complex. Owing to low sun elevation angles and the lack of seasons in these areas, combined with rugged topography, this may lead to Permanently Shadowed Regions (PSRs) in craters and topographic depressions, where low temperatures allow ice to accumulate [1]. In contrast, Long-term Illuminated Areas (LIAs) on high-standing ridges and crater rims enable almost uninterrupted illumination and solar power supply [2]. High-resolution Digital Terrain Models (DTMs) are crucial for modelling these illumination conditions and for general support of future polar exploration missions [3]. We choose to derive those models from images captured by the Lunar Reconnaissance Orbiter (LRO) Narrow Angle Camera (NAC) for LIAs and by ShadowCam for PSRs [4], [5]. Here, we use our deep learning method developed previously to derive south pole DTMs, which can achieve a similar or even better effective resolution to those produced by the SFS method [6], stereo photogrammetry, or laser altimetry. We selected Shackleton Crater (a typical PSR) and Malapert Massif (a candidate landing site for the Artemis Program) as experimental areas to derive DTMs with resolutions of 2 meters and 1 meter, respectively. Finally, we used the DTMs to perform refined illuminated modeling and analysis to support future lunar south pole exploration missions.

 

References:

[1] Brown, H.M., et al. (2022) Resource potential of lunar permanently shadowed regions. Icarus, 377, p.114874.

[2] Gläser, P., et al. (2018) Illumination conditions at the lunar poles: Implications for future exploration. Planetary and Space Science, 162, pp.170-178.

[3] Chen, H., et al. (2022) CNN-based large area pixel-resolution topography retrieval from single-view LROC NAC images constrained with SLDEM. IEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing, 15, pp.9398-9416.

[4] Robinson, M.S., et al. (2010) Lunar reconnaissance orbiter camera (LROC) instrument overview. Space Science Reviews, 150, pp.81-124.

[5] Robinson, M.S., et al. (2023) ShadowCam instrument and investigation overview. Journal of Astronomy and Space Sciences, 40(4), pp.149-171.

[6] Chen, H., et al. (2024) ELunarDTMNet: Efficient reconstruction of high-resolution lunar DTM from single-view orbiter images. IEEE Transactions on Geoscience and Remote Sensing, 62, pp. 1-20.

How to cite: Chen, H., Gläser, P., Willner, K., Huang, Q., Xie, X., and Oberst, J.: High-resolution Topographic Modeling for the Lunar South Pole Region Using NAC and ShadowCam Images, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3321, https://doi.org/10.5194/egusphere-egu25-3321, 2025.

EGU25-5037 | ECS | Posters on site | PS7.5

Mercury's annual and long-term librations from self-registration of MLA profiles  

Haifeng Xiao, Alexander Stark, Stefano Bertone, Attilio Rivoldini, Rose-Marie Baland, Marie Yseboodt, Oliver Stenzel, Arthur Briaud, Hauke Hussmann, Luisa Lara, and Pedro Gutiérrez

Mercury's annual longitudinal libration (88 days) and its mean rotation rate have been  determined based on independent observations from the ground-based radar (Margot et al., 2012), camera and/or laser altimetry (Stark et al., 2015; Bertone et al., 2021), and radio science (Mazarico et al., 2014; Genova et al., 2019; Konopliv et al., 2020). Although consistent, the precision of the libration measurements precludes identification of a large solid inner core (Van Hoolst et al., 2012). At the same time, the measured rotation rates are largely inconsistent. Deviation from the resonant rotation rate is caused by the planet-induced long-term librations which can be amplified if their periods are close to that of a free libration mode (Yseboodt et al., 2013).

We devise an alternative and innovative approach aimed at precisely tracking how the rotation angle varies with time so that various libration terms can be analyzed quantitatively. The approach involves two self-registration processes of the MESSENGER Mercury Laser Altimeter (MLA) profiles (Xiao et al., 2024). We focus on a small polar region from 81°N to 84°N. In the first step, we carry out the self-registration by shifting the individual profiles laterally and radially to get rid of the slow-varying orbit, pointing, and timing errors, which can be treated as near-constant. In contrast to the aforementioned near-constant shifts, offsets in the rotation angles can lead to non-linear rotation-like distortions of the profiles. Offsets in the orientation angles of the spin axis can shift the profiles as a whole, ensuring that our approach is insensitive to the a priori orientation state. Then in the second step, we update the inertial coordinates of the profiles and perform the second self-registration in which adjustments are made to the rotation angles at the acquisition times of each of the profiles. However, as the periapsis of the spacecraft has drifted throughout the mission, the ground track does not exactly cross the North Pole and an offset in the rotation angle can also shift the centroid of the profile. In the light of this, the above two-step process needs to be iterated till convergence. Finally, we obtain the updated rotation angle per profile uncontaminated by external error sources.

We have experimented with various a priori rotation and orientation values, i.e., Stark2015, IAU2015 (Archinal et al., 2018), Genova2019, and Bertone2021. An example of the obtained variation of the rotation with time is shown in Figure 1. The long-term libration most likely to be amplified and captured is that with a period of around 6 years, induced by Venus (5.66 y), or by Jupiter (5.93 y), or by the Earth (6.57 y). The superposition of multiple long-period terms is also possible. We will carry out close-loop simulations to assess uncertainty and consider interior and libration modelings to interpret the scientific implications.

Figure 1: Rotation variation with time using the IAU2015 model as a priori values. Correction is with respect to Mercury’s resonant rotation.

References:

Archinal et al., 2018. Celest. Mech. Dyn. Astron.. Bertone et al., 2021. JGR. Mazarico et al., 2014. JGR. Genova et al., 2019. GRL. Konopliv et al., 2020. Icarus.  Margot et al., 2012. JGR.  Stark et al., 2015. GRL.  Van Hoolst et al., 2012. EPSL. Xiao et al., 2024. Authorea Preprints. Yseboodt et al., 2013. Icarus.

How to cite: Xiao, H., Stark, A., Bertone, S., Rivoldini, A., Baland, R.-M., Yseboodt, M., Stenzel, O., Briaud, A., Hussmann, H., Lara, L., and Gutiérrez, P.: Mercury's annual and long-term librations from self-registration of MLA profiles , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5037, https://doi.org/10.5194/egusphere-egu25-5037, 2025.

EGU25-6291 | ECS | Posters on site | PS7.5

Quantifying the size of impact basins through analysis of gravity and crustal thickness data 

Salvatore Buoninfante, Mark A. Wieczorek, Valentina Galluzzi, Luigi Ferranti, Maurizio Milano, Maurizio Fedi, and Pasquale Palumbo

The surface and crustal structure of the terrestrial planets in the inner solar system have been influenced by large and energetic impact events. GRAIL data showed that the size of the central gravitational anomaly of lunar basins corresponds closely to the diameter of the inner peak-ring [1].

We present an improved technique based on the analysis of gravity and crustal thickness data to estimate the inner ring and rim crest diameters. This technique expands upon the work of [1] and allows us to better identify highly degraded basins. From this analysis, we also quantify how lower resolution gravity and crustal thickness datasets (such as for Mars and Mercury) might bias the peak ring and main rim diameter estimates.

In our approach, we first quantify the regional value of the Bouguer gravity anomaly and crustal thickness, which is defined as the average value obtained from azimuthally averaged profiles in the radius range 1.5 D to 2 D, where D is the crater diameter. The diameter of the Bouguer gravity high, as well as the diameter of the crustal thickness anomaly, were then estimated as the radius where the profiles first intersect the background regional values. After the initial estimate of D was obtained, the procedure was iterated until there was no change in the obtained diameters.

We tested this method using Bouguer gravity data for certain lunar peak-ring and multi-ring basins, by considering the spherical harmonic degree range from 6 to 540. We then filtered the data using the spherical harmonic degree range 6-49 in order to simulate the lower resolution of the Mars gravity models (e.g., [2]). We then used the same approach using crustal thickness maps derived after GRAIL [3], both for the degree ranges 6-310 and 6-46, to simulate the loss of spatial resolution of Mars [4]. Uncertainty estimates were obtained for the crustal thickness and the Bouguer anomaly diameter by considering the ±1σ values for the background values in the spatial range of 1.5 D to 2 D.

Our method properly detects peak-ring or inner ring sizes for lunar basins with main rim diameter greater than 250 km. Nevertheless, when considering filtered versions of these datasets that correspond to the effective spatial resolution of the Mars gravity models, only basins with rim crest diameters greater than about 450 km can be detected with acceptable accuracy. Finally, results from these analyses will allow us to better constrain the impact rate during the early solar system.

 

​​​​​​

References:

[1] Neumann G. A., et al. (2015). Sci. Adv.

[2] Genova A., et al. (2016). Icarus.

[3] Wieczorek M. A., et al. (2013). Science.

[4] Wieczorek M. A., et al. (2022). JGR: Planets.

 

Acknowledgements: We gratefully acknowledge funding from the Italian Space Agency (ASI) under ASI-INAF agreement 2024-18-HH.0.

 

How to cite: Buoninfante, S., Wieczorek, M. A., Galluzzi, V., Ferranti, L., Milano, M., Fedi, M., and Palumbo, P.: Quantifying the size of impact basins through analysis of gravity and crustal thickness data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6291, https://doi.org/10.5194/egusphere-egu25-6291, 2025.

EGU25-6513 | ECS | Orals | PS7.5

Magnetic signature of La Corona lava tube (Lanzarote, Canary Islands) as a planetary analog 

Juan Martin de Blas, Yasmina M. Martos, Jared Espley, Jacob Richardson, Dave Sheppard, and John Connerney

The island of Lanzarote (Canary Islands) is widely recognized as a terrestrial analog for planetary science due to its geological and environmental characteristics. This island hosts numerous lava tubes, including the 7.6-km-long La Corona tube, one of Earth’s largest. Detecting lava tubes and other subsurface cavities is crucial for planetary exploration, as they may be used as safe shelters in future planetary missions. 


Magnetic data, including scalar and vector magnetometer data as well as magnetic susceptibility measurements, were collected during the NASA Goddard GeoLife expedition in May 2023 to study three lava tubes of different morphometry, age, and geological features: La Corona, Los Naturalistas, and Tahiche. This study focuses on analyzing vector magnetometer measurements over La Corona tube. We rotate and process the vector magnetic measurements to derive magnetic anomalies of both the total magnetic field and the individual vector components. To identify, delineate, and characterize the lava tube, we apply various enhancement techniques such as calculating the reduction to the pole or the lateral derivatives.


Our findings reveal the feasibility of using vector magnetometer data to detect lava tubes. Additionally, we show that our magnetic anomaly values derived from vector magnetometer data are comparable to those obtained from scalar magnetometer data. Lastly, we illustrate that we can extract valuable information from each of the vector magnetic field components and use them together with the total field values to identify and interpret magnetic subsurface features.

How to cite: Martin de Blas, J., Martos, Y. M., Espley, J., Richardson, J., Sheppard, D., and Connerney, J.: Magnetic signature of La Corona lava tube (Lanzarote, Canary Islands) as a planetary analog, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6513, https://doi.org/10.5194/egusphere-egu25-6513, 2025.

EGU25-8720 | ECS | Posters on site | PS7.5

Planetary Interior Modeling Using Synthetic Gravity Simulator 

Edoardo Santero Mormile and Giuseppe Mitri

Gravity inversion techniques enable the characterisation of the internal mass distribution of planetary bodies by combining data from their shape, gravity, and rotation. However, the inherent ambiguity in scalar gravity signals, specifically, between mass and depth, poses a significant challenge for inferring internal structure. In this work, we introduce a novel approach leveraging the spherical harmonics framework described in [1], in particular, the gravitational harmonics coefficients [Cnm, Snm]. Starting with a simplified interior structure (assuming homogeneous layers), interior model parameters are the number of layers, average layer thickness, average layer density, and the topography of layer interfaces (if present). Regarding the latter, in cases where Bouguer anomalies are available, the mantle-crust interface topography can be inferred using a filtering approach, as proposed in [2]. Notably, this method does not rely on assumptions of isostatic compensation but requires careful selection of the filtering parameters. From these parameters. the spherical harmonics coefficients for each layer and the global ones are computed (see [1]). From these coefficients, key quantities such as gravitational potential, Free-Air anomalies, and Bouguer anomaly maps are evaluated and then compared to space measurements, measuring the model performance by different metrics (e.g. RMSE, structural similarity index, Pearson correlation coefficient). By varying model parameters randomly within physically constrained ranges (e.g. by mass conservation, moment of inertia and observed shape), this process is repeated iteratively. The parameter combination minimizing the performance metrics between modelled and observed data represents the best-fit internal structure. This approach is robust and flexible at the same time, being able to accommodate diverse celestial bodies with a wide variety of planetary shapes, internal configurations, and gravitational data sets and to objectively identify the optimal parameter configuration. This method is benchmarked on Mercury [3], resulting in a mantle-crust interface at ~28 km depth and a mantle density of 3210 [kg/m3], consistent with existing literature (see [4]). Furthermore, this procedure can be used to compute the expected gravity signal from unknown bodies targeted by the upcoming missions and instruments (e.g. Ganymede for JUICE), test different theoric interior models, and obtain their gravitational response.

Acknowledgements: ESM and GM acknowledge support from the Italian Space Agency (2022-16-HH.1-2024). This paper and related research have been conducted during and with the support of the Italian national inter-university PhD programme in Space Science and Technology.

References: [1] M. A. Wieczorek, ‘Gravity and Topography of the Terrestrial Planets’, in Treatise on Geophysics, Elsevier, 2015, pp. 153–193. doi: 10.1016/B978-0-444-53802-4.00169-X.[2] M. A. Wieczorek and R. J. Phillips, ‘Potential anomalies on a sphere: Applications to the thickness of the lunar crust’, Journal of Geophysical Research: Planets, vol. 103, no. E1, pp. 1715–1724, 1998, doi: 10.1029/97JE03136.[3] A. Genova et al., Regional variations of Mercury’s crustal density and porosity from MESSENGER gravity data, Icarus, vol. 391, p. 115332, Feb. 2023.[4] S. Buoninfante, M. Milano, B. Negri et al. ‘Gravity evidence for a heterogeneous crust of Mercury’. Sci Rep 13, 19854 (2023), https://doi.org/10.1038/s41598-023-46081-4

How to cite: Santero Mormile, E. and Mitri, G.: Planetary Interior Modeling Using Synthetic Gravity Simulator, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8720, https://doi.org/10.5194/egusphere-egu25-8720, 2025.

EGU25-8998 | Orals | PS7.5

Benchmarking dynamic topography across geodynamical codes 

Cedric Thieulot, Olga Ortega-Gelabert, Bart Root, and Clinton Conrad

During the ESA funded 4D Dynamic Earth project, different sensitivity studies are performed to understand the applicability of current ground and satellite datasets available to study the dynamical behavior of the solid Earth, in particular the complete mantle. This project is a joint effort between ESA and many European universities and is lead by Delft University of Technology (https://4ddynamicearth.tudelft.nl/). 

The project consists of ten work packages, many of them relying on some form of forward geodynamical modelling. Given the diversity of participants multiple codes are used in the project: a 2D axisymmetric Python code developed by C.T. at the Utrecht University, a 3D Matlab code developed by O.O-G. and the 3D massively parallel C++ community code ASPECT.

One recurring quantity that is of paramount importance for some work packages is dynamic topography, i.e. the outer surface expression to dynamic mantle flow. We have therefore designed a simple isothermal experiment of an anomalous sphere present in the mantle of a planet (the core is ignored as is customary in whole-Earth geodynamic modelling). The sphere itself can be positively or negatively buoyant, and the mantle can be isoviscous or characterized by a radial viscosity profile. Boundary conditions at the core-mantle boundary and at the surface are either no-slip or free-slip. 

Dynamic topography calculations involve the radial stress which is derived from the primitive variables velocity (actually, its gradient) and pressure which are found to be sensitive to mesh size in both radial and lateral directions. We therefore report on the root mean square velocity, the surface strain rate, stress and dynamic topography and the gravity anomaly for a range of experiments. Our objective is two-fold: characterize the accuracy of our codes and provide the community with a benchmark. 

All three codes are Finite Element codes and all rely on the Taylor-Hood element but they are also quite different with respect to meshing and solver architecture. Nevertheless we find that all measured quantities converge within approx. 1% for radial resolutions of at least 30km.

How to cite: Thieulot, C., Ortega-Gelabert, O., Root, B., and Conrad, C.: Benchmarking dynamic topography across geodynamical codes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8998, https://doi.org/10.5194/egusphere-egu25-8998, 2025.

EGU25-10169 | ECS | Posters on site | PS7.5

Quantifying Mercury's tidal response: A framework for understanding planetary interiors 

Arthur Briaud, Alexander Stark, Hauke Hussmann, Haifeng Xiao, and Jürgen Oberst

Mercury's unique orbital dynamics, influenced by its proximity to the Sun and high eccentricity, lead to periodic variations in tidal forces and surface temperature patterns. The tidal Love numbers (TLNs), which characterize the planet's deformation and gravitational field changes, are highly sensitive to key internal parameters such as core size, mantle composition and rheology, and the presence of lateral and vertical heterogeneities e.g., [1-5]. Mercury's TLNs thus provide a quantitative framework for understanding how its internal structure responds to tidal forces. In this study, we systematically investigate how variations in these internal parameters affect Mercury's TLNs. We use numerical models to simulate the tidal response of the planet, taking into account a wide range of geophysical and thermodynamic conditions. In particular, we investigate the effects of core-mantle interactions, variations in mantle viscosity and temperature, and potential anisotropies within the lithosphere. Our results show that TLNs are particularly influenced by the size and state of the core, the thermal gradient across the mantle, and the degree of lateral heterogeneity within the inner layers. To validate and refine our models, we will integrate these results with observational constraints such as Mercury's mean density, moment of inertia, and surface deformation data e.g., [1, 6]. This study will provide important insights for interpreting future high-precision measurements from the BepiColombo mission [7]. By linking TLNs to Mercury's internal parameters, we aim to develop a robust framework for constraining the planet's internal structure, providing a deeper understanding of its geodynamic evolution and its significance in the broader context of the formation and evolution of terrestrial planets.

References:

[1] Goossens et al., 2022. The Planetary Science Journal, 3(6), 145.

[2] Mazarico et al., 2014. Journal of Geophysical Research: Planets, 119(12), 2417-2436.

[3] Mosegaard and Tarantla, 1995. Journal of Geophysical Research: Solid Earth, 100(B7), 12431-12447.

[4] Steinbrügge et al., 2018. Journal of Geophysical Research: Planets, 123(10), 2760-2772.

[5] Rivoldini et al., 2009. Icarus, 201(1), 12-30.

[6] Genova et al., (2019), Geophysical Research Letters, 46(7), 3625-3633.

[7] Hussmann and Stark, (2020), The European Physical Journal Special Topics, 229, 1379-1389.

How to cite: Briaud, A., Stark, A., Hussmann, H., Xiao, H., and Oberst, J.: Quantifying Mercury's tidal response: A framework for understanding planetary interiors, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10169, https://doi.org/10.5194/egusphere-egu25-10169, 2025.

EGU25-10842 | Orals | PS7.5

Geophysical investigation of the terrestrial analogue, Caldereta volcano, in Lanzarote, the Canary Islands as a precursory study to mars phreatomagmatic volcanoes 

Marina Díaz-Michelena, Emma Losantos, Miguel Ángel Rivero, Joana S. Oliveira, Óscar García Monasterio1, Federico Mansilla, Ángel Melguizo, José Luis García Bueno, David Salamanca, and Sergio Fernández Romero

Hydromagmatic eruptions are of particular importance for the search of extraterrestrial life since they require the presence of water. Phreatomagmatic volcanoes on Mars shall resemble those of the Earth and thus, terrestrial analogues of Mars, such as Lanzarote in the Canary Islands, are a good reference for further studies of the Martian volcanoes.

In this study we present our drone-based magnetic survey results combined with a morphometric analysis of Caldereta horse-shoe shaped volcano in Lanzarote, catalogued as a phreatomagmatic tuff for its similarity and proximity to Caldera Blanca, a well-known hydromagmatic edifice (Barrera Morate et al., 2011; Carracedo and Day, 2002; Romero et al., 2007; Kervyn et al., 2012; Brož and Hauber, 2013). On Mars, the chosen edifice is C27 volcano, a horse-shoe shaped cone in the Nephentes/Amenthes region, whose pitted cones were suggested to be of phreatomagmatic origin by Brož and Hauber (2013).

Our morphometric analyses allowed us to classify both Caldereta and C27 edifices as tuff rings, specifically maars. With the drone-based survey performed in Caldereta we demonstrate how more insights could be gained from Martian volcanos when combining magnetic surveys using helicopters on Mars (Mittelholz et al., 2023) with morphometric analyses using satellite data and high-resolution near surface geophysical studies.

 

Keywords

Magnetometry, Mars, planetary magnetism, crustal magnetism, Mars hydromagmatism, planetary science, space magnetometers.

 

References:

Barrera Morate J.L., García Moral R., 2011. Mapa geológico de Canarias. GRAFCAN.  https://www.idecanarias.es/resources/GEOLOGICO/LZ_LITO_unidades_geologicas.pdf

Brož, P., Hauber, E., 2013. Hydrovolcanic tuff rings and cones as indicators for phreatomagmatic explosive eruptions on Mars. J. of Geophys. Res.: Planets 118, 1656–1675. doi: 10.1002/jgre.20120.

Carracedo, J.C., Day, S., 2002. Canary Islands, in: Classic Geology in Europe Series 4. Terra Publishing, Harpenden, Hertfordshire, p. 294.

Kervyn, M., Ernst, G.G.J., Carracedo, J.C., Jacobs, P., 2012. Geomorphometric variability of “monogenetic” volcanic cones: Evidence from Mauna Kea, Lanzarote and experimental cones. J. Geomorphol. 136, 59-75. https://doi.org/10.1016/j.geomorph.2011.04.009

Mittelholz, A., Heagy, L., Johnson, C. L., Fraeman, A. A., Langlais, B., Lillis, R. J., and Rapin, W.: Helicopter Magnetic Field Surveys for Future Mars Missions, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-11186, https://doi.org/10.5194/egusphere-egu23-11186, 2023.Romero, C., Dóniz, J., García Cacho, L., Guillén, C., Coello, E., 2007. Nuevas evidencias acerca del origen hidromagmático del conjunto volcánico Caldera Blanca/Risco Quebrado (Lanzarote, Islas Canarias). Resúmenes XII Reunión Nacional de Cuaternario, Ávila.

How to cite: Díaz-Michelena, M., Losantos, E., Rivero, M. Á., Oliveira, J. S., García Monasterio1, Ó., Mansilla, F., Melguizo, Á., García Bueno, J. L., Salamanca, D., and Fernández Romero, S.: Geophysical investigation of the terrestrial analogue, Caldereta volcano, in Lanzarote, the Canary Islands as a precursory study to mars phreatomagmatic volcanoes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10842, https://doi.org/10.5194/egusphere-egu25-10842, 2025.

EGU25-11941 | Posters on site | PS7.5

How tidal tomography and thermal constraints can probe the existence of a Martian basal molten layer 

Clément Ganino, Alex Guinard, Agnès Fienga, and Anthony Mémin

By computing the tidal deformations of Mars, we investigated its spherically symmetric internal structure, and specifically the nature (liquid, partially melted or both) of the interface between the mantle and the liquid core. Through an evaluation of their compatibility with diverse geophysical observations, we demonstrated that, despite the short excitation periods, tidal deformation (tidal dissipation induced by Phobos and tidal quality factor at the Phobos excitation frequency) provides an effective means to constrain Mars's internal structure. Our analysis yielded independently density and thickness estimates for the Martian lithosphere, mantle, core–mantle boundary layers, and core, which were consistent with previous results from other methods. Additionally, we derived new viscosity estimates for these layers. Notably, we showed that geodetic observations, combined with thermal constraints, are particularly sensitive to the presence of a two-layered interface at the top of the liquid core in the deep Martian mantle. This interface comprises two layers with similar densities but very different viscosities and rheologies. The layer directly atop the liquid core follows a Newtonian constitutive equation (Newtonian Basal Layer or NBL), while the overlying layer at the base of the mantle has an Andrade rheology (Andrade Basal Layer or ABL), characterized by a viscosity approximately 10 orders of magnitude greater than that of the Newtonian layer. Our results indicate that the presence of this two-layered interface significantly affects the viscosity profiles of both the mantle and lithosphere. Specifically, models incorporating the two-layered interface show small viscosity contrast between the mantle and the lithosphere, preventing mechanical decoupling between these layers. This would support a stagnant lid regime, consistent with the current absence of Earth-like plate tectonics on Mars. Finally, our findings suggest that the presence of a liquid Newtonian layer atop the liquid core is incompatible with the existence of a solid inner core on Mars.

How to cite: Ganino, C., Guinard, A., Fienga, A., and Mémin, A.: How tidal tomography and thermal constraints can probe the existence of a Martian basal molten layer, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11941, https://doi.org/10.5194/egusphere-egu25-11941, 2025.

EGU25-12405 | Posters on site | PS7.5

VERITAS Gravity Science Experiment: Impact of Colored Noise on Parameter Estimation 

Fabrizio De Marchi, Flavia Giuliani, Daniele Durante, Gael Cascioli, Luciano Iess, Erwan Mazarico, and Suzanne Smrekar

The VERITAS (Venus Emissivity, Radio Science, InSAR, Topography, and Spectroscopy) mission is a future NASA Discovery mission that aims to improve our understanding of Venus' evolution, structure, and geological processes. Its gravity science experiment will produce a uniform, high-resolution gravity map of Venus, providing unprecedented constraints on the planet’s crustal and interior structure. The radio tracking relies on a dual-frequency transponder in X and Ka bands. This advanced multi-frequency system achieves Doppler measurement accuracy of about 18 μm/s (for most of the mission duration) at 10-second integration time and can correct 75% of the plasma noise, particularly important at low Sun-Probe-Earth (SPE) angles (<15-20°).

Numerical simulations of the VERITAS gravity experiment were carried out using JPL’s MONTE software, considering detailed dynamical and noise models. The noise model accounts for 1) media propagation effects, i.e., troposphere, ionosphere, and plasma, where troposphere has a seasonal variation and plasma noise depends on SPE angle, and 2) spacecraft and ground station instrumentation. While many noise sources have a white noise spectral profile, significant contributors such as the frequency and timing system (FTS) and plasma introduce colored noise, i.e., whose magnitude varies with frequency.

A colored-noise results in a non-diagonal correlation matrix which can bias (with respect to a white-noise case) the best-fit estimated parameters and lead to an underestimation of their uncertainties.

Therefore, the main objective of this work is to evaluate the impact of colored noise on the estimation of the parameters related to the Venus’ gravity field (i.e., the spherical harmonic coefficients).

To this aim, we simulated the Doppler observables and the gravity recovery for both the white-noise and colored-noise cases. Colored noise was simulated with the algorithm described by [1] and we developed a method to incorporate these correlations into the sequential filtering process used for orbit determination. We will present the results of these simulations.

[1] Timmer, J. and Koenig, M. (1995). On generating power law noise. Astronomy and Astrophysics, 300:707.

How to cite: De Marchi, F., Giuliani, F., Durante, D., Cascioli, G., Iess, L., Mazarico, E., and Smrekar, S.: VERITAS Gravity Science Experiment: Impact of Colored Noise on Parameter Estimation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12405, https://doi.org/10.5194/egusphere-egu25-12405, 2025.

EGU25-12535 | ECS | Orals | PS7.5

COMPARATIVE ANALYSIS OF YOLOv8 AND YOLOv11 FOR COLD SPOT DETECTION ON THE LUNAR SURFACE 

Shachaf Weil Zattelman and Fadi Kizel

Lunar cold spots are thermal anomalies associated with fresh impact craters and understanding them offers critical insights into the Moon's surface evolution and thermophysical properties. Traditionally, their detection has relied on manual methods, which are labor-intensive and time-consuming. This study evaluates the performance of two advanced deep learning-based object detection models, YOLOv8 and YOLOv11, for automating lunar cold spot detection using Diviner radiometer data. The training dataset was generated from 128-pixel-per-degree (ppd) rock-free nighttime regolith temperature maps covering latitudes up to ±60°. The dataset included 384 lunar images with 652 annotated cold spots for model training. For testing, the 2023 High-Resolution Nighttime Temperature dataset was cropped into 512×512-pixel sub-images (~4×4 degrees) with a 20% overlap to capture edge cold spots. This process generated 4,816 sub-images, ensuring comprehensive coverage and minimizing missed detections.

The experimental design included two strategies: a straightforward train-test split and a more robust 5-fold cross-validation approach. The models were assessed using key performance metrics: precision, recall, F1 score, and mean Average Precision (mAP). YOLOv11 consistently outperformed YOLOv8 across most metrics, achieving a precision of 0.85, recall of 0.78, F1 score of 0.81, and mAP-50 of 0.79 with K-fold cross-validation. Both models demonstrated superior performance in detecting faint thermal anomalies, showcasing their capability to identify subtle features often overlooked by manual methods.

Hyperparameter tuning and robust preprocessing techniques, including overlapping sub-image and data augmentation, contributed significantly to the models' performance. YOLOv11's higher selectivity resulted in fewer false positives and greater reliability, whereas YOLOv8 identified a larger number of cold spots, though with a higher false positive rate. Both models significantly outperformed manual detection methods, demonstrating their ability to expand the catalog of lunar cold spots efficiently and accurately with precision of 78% and 89% for YOLOv8 and Yolov11, respectively. This automated approach identified previously undetected cold spots, providing a more comprehensive understanding of lunar thermal anomalies and their spatial distribution.

These findings highlight the transformative potential of convolutional neural networks (CNNs) in planetary science, particularly in automating complex and data-intensive tasks like lunar cold spot detection. The scalability and precision of YOLOv11, combined with YOLOv8's sensitivity to faint anomalies, underscore the value of integrating deep learning techniques into planetary exploration and research.

How to cite: Weil Zattelman, S. and Kizel, F.: COMPARATIVE ANALYSIS OF YOLOv8 AND YOLOv11 FOR COLD SPOT DETECTION ON THE LUNAR SURFACE, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12535, https://doi.org/10.5194/egusphere-egu25-12535, 2025.

EGU25-13284 | ECS | Orals | PS7.5

Geochemical and Mineralogical Signatures of Alluvial Fans in Iceland and their Implications for Late Stage Aqueous Activity on Mars 

Amanda Rudolph, James Haber, Sharon Wilson, Rossman Irwin, Alexander Morgan, Briony Horgan, Timothy Rose, and Rob Wardell

Extensive physical and chemical evidence from orbiter, lander, and rover data show that surface water was widespread on Mars into the Amazonian. Alluvial fans are geologic landforms on Mars that preserve evidence of this late-stage aqueous activity in the geologic record. The composition and distribution materials in an alluvial fan, either in the catchment (source) and/or the fan (sink), help inform our understanding of the origin and extent of aqueous alteration, either in the source rocks prior to deposition or after, in the fan itself. However, the geochemical and mineralogical properties of martian alluvial fans, and how these properties vary from the catchment to the fan, are not well constrained. 

The work presented here characterizes the geochemistry and mineralogy of two alluvial fans and their associated catchments at sites in Iceland—Fjallabak and near Hoffellsjökull—which serve as close compositional analogs for Mars. These results can help us to understand the aqueous alteration that formed similar deposits on Mars while placing constraints on martian geologic history and paleoclimate.

We utilize a suite of complementary laboratory techniques: Raman spectroscopy, scanning electron microscopy with an energy dispersive X-ray detector (SEM/EDS), and X-ray diffraction (XRD). Raman spectroscopy qualitatively maps spectral properties to confirm existing mineral identification and spectra are processed to determine the relative abundance materials; this technique is of particular use to identify amorphous glass. SEM/EDS is used to quantitatively map elemental compositions, and XRD with Rietveld refinement can identify the type and abundance of crystalline minerals. Raman and XRD both have in situ instrument analogs on the surface of Mars: the Scanning Habitable Environments with Raman and Luminescence for Organics and Chemicals (SHERLOC) on the Perseverance rover, and Chemistry and Mineralogy (CheMin) instrument on the Curiosity rover, respectively. SEM/EDS techniques are also likely to be applied to samples returned from Mars.

At Fjallabak, source rocks are primarily a combination of hyaloclastite (a product of subglacial volcanism) and rhyolite. At Hoffellsjökull, the rocks are mostly basalt with evidence of minor hydrothermal alteration. Rocks and sediments do not appear to be heavily altered upon deposition into the alluvial fan, although some authigenic alteration may have occurred in the catchment itself.

Preliminary Raman spectral analyses support our initial field interpretations of the rocks and minerals observed at both field sites. To date, we have analyzed hyaloclastite source rocks and confirmed the presence of obsidian and/or albite glass, along with signs of aqueous alteration indicated by Fe-oxides (i.e., goethite) at Fjallabak. We have also identified diopside (Ca-Mg clinopyroxene) and actinolite (a low-grade metamorphic mineral) in inferred hydrothermally altered basalt, along possible Fe-oxide-hydroxides (i.e., lepidocrocite) that indicate aqueous alteration in the Hoffellsjökull fan. Initial results suggest aqueous alteration of materials at both field sites but the distribution of primary versus secondary materials has yet to be constrained. 

Our results will include the laboratory analysis that characterize these Iceland fans that will help determine the extent and distribution of alteration products in alluvial fans at Mars compositional analog sites.

How to cite: Rudolph, A., Haber, J., Wilson, S., Irwin, R., Morgan, A., Horgan, B., Rose, T., and Wardell, R.: Geochemical and Mineralogical Signatures of Alluvial Fans in Iceland and their Implications for Late Stage Aqueous Activity on Mars, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13284, https://doi.org/10.5194/egusphere-egu25-13284, 2025.

EGU25-13316 | ECS | Orals | PS7.5

Using Remote Sensing to Understand Icelandic Alluvial Fan Composition as an Analog for a Cold and Wet Ancient Mars 

James Haber, Amanda Rudolph, Rossman Irwin, Alexander Morgan, Briony Horgan, and Sharon Wilson

Fan-shaped deposits, including alluvial fans and deltas, are abundant on Mars. They preserve evidence of episodic running water and potentially habitable environments into the early Amazonian. Most alluvial fan analog studies have focused on depositional processes, rather than the composition of fan materials. In particular, it is unclear if the composition of fan deposits represents alteration during transport/deposition or the composition of the watershed in a cold environment.

In this study, we use a suite of remote sensing techniques to characterize mineralogy of rocks and sediments in alluvial fans in Iceland to understand any distinct trends within this tundra climate. This work helps fill a knowledge gap for understanding alluvial fans on Mars through the novel analog study in a cold climate on Earth. Iceland has been widely studied as a Mars analog because of its dominant basaltic composition, general lack of vegetation, and tundra climate. We analyze several alluvial fans of variable morphology, location, and composition to understand how these factors might affect the alteration of fan sediments.

Prior to fieldwork, we analyzed high-resolution orbital images (15 m/pixel) from the World Imagery ESRI Basemap and spectral data (10-60 m/pixel) from the SENTINEL-2 MultiSpectral Instrument in the visible to near infrared (VNIR) range (13 bands; 0.443-2.190 μm) to characterize decameter-scale compositional variability. 

During our July 2024 field season, we imaged fans and their watersheds using a DJI Mavic Pro 2 drone at the meter- to decameter-scale. We used a portable ASD QualitySpec Trek spectrometer to collect VNIR (0.35-2.5 μm) reflectance spectra and identify minerals along transects from the fan apex to toe to capture compositional variability in the fan deposits and their watersheds.

Our results focus on two alluvial fans and their watersheds: one dominated by rhyolite and hyaloclastite in Fjallabak Nature Reserve in the Icelandic highlands and another dominated by basalt near Hoffellsjökull in eastern Iceland. In VNIR spectra from Fjallbak, we observe absorption bands due to hydration (1.4 and 1.9 μm), Fe-oxides (0.53 and ~0.9 μm), and hydrated silica (2.2 μm). At Hoffellsjökull, we also observe kaolinite (2.2 μm doublet) in tan rocks and calcite (2.338 μm) in veins and vesicles within basalt. We also observe broad absorptions near 1 and 2 μm likely due to primary mafic minerals such as olivine, pyroxene, or volcanic glass.

Our results indicate that rocks in the alluvial fans were sourced from a variety of lithologies, which we are able to identify in the watershed using drone and orbiter images. Overall, we do not observe major differences in composition between the fan deposits and their watersheds, suggesting that there is minimal alteration during transport and deposition. Ongoing work includes detailed spectral analyses of sediments along fan transects and comparisons to the watershed to determine how the rocks and sediments vary across the fan deposit. Additionally, comparisons to similar alluvial fans on Mars will improve our understanding of how these features may have formed in a cold climate.

How to cite: Haber, J., Rudolph, A., Irwin, R., Morgan, A., Horgan, B., and Wilson, S.: Using Remote Sensing to Understand Icelandic Alluvial Fan Composition as an Analog for a Cold and Wet Ancient Mars, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13316, https://doi.org/10.5194/egusphere-egu25-13316, 2025.

EGU25-17694 | ECS | Posters on site | PS7.5

Unravelling similarities between Mount Etna's pyroclastic deposits and the Lunar counterparts. 

Giacomo Melchiori, Matteo Massironi, Riccardo Pozzobon, Patrizia Ferretti, and Sonia Calvari

In the last few years, NASA, ESA, CNSA and JAXA have been planning comprehensive lunar initiatives, including the Artemis program. In this context, it is crucial to i) support scientific research aimed at improving our ability to collect direct ground-truth data and samples, and ii) test equipment and validate analytical methodologies at designated analogue sites. Among the sites of interest on the lunar surface are the ones dominated by pyroclastic deposits since, as shown on Apollo samples, they may have trapped considerable volumes of gases3, being their formation linked to the presence of volatiles within magma. This material represent an intriguing in-situ resource1 that has yet to be verified even considering studies on Earth analogues on volcanic environments. Some of them are well internationally-known (e.g., Lanzarote, Canary Islands4; Kilauea Volcano, USA; Lava Beds National Monument, USA)  and have been extensively studied. In other cases, such as Mount Etna, the compositional similarity remains unexplored, despite the site has already attracted interest from the planetary science community2. Mount Etna volcano exhibits several geological similarities with lunar features such as the presence of  lava tubes, cinder cones, lava channels and bowl shaped pits; however, its analogy from a compositional point of view has yet to be determined.

For this reason, several unweathered and unaltered  samples have been collected from a pyroclastic deposit in the area of the Cisternazza pit crater, a collapse pit located on the southern flank of Mount Etna. The samples underwent comprehensive chemical and mineralogical characterization, revealing compositional similarities with lunar samples. Consequently, further tests were conducted to examine their mechanical, thermal, and spectral behaviour to compare it with lunar samples and certified lunar simulants across a broader range of properties.

To assess the analogy with the lunar surface, specific spectral parameters were also calculated for both the Etna samples and key sites on the Moon. In addition, in order to resemble the complex spectral response of the lunar pyroclastic deposits, we generated different mixtures using the spectra of the Etna samples intermixed with different amounts of olivine, orthopyroxene, and clinopyroxene endmembers spectra. Intriguing correlations between these mixtures and lunar spectral data were observed, even in study areas far from Apollo landing sites, indicating a broader range of similarities with the lunar pyroclastic materials.

Acknowledgement

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 n. 2024-5-E.0 - CUP n. I53D24000060005.

References

1: Anand et al., 2012, A brief review of chemical and mineralogical resources on the Moon and likely initial in situ resource utilization (ISRU) applications. Planet. Space Sci. 74, 42–48.

2: Carey et al., 2022, METERON Analog-1: A Touch Remote. 73rd International Astronautical Congress (IAC), Paris, France, 18–22 September 2022

3: Ivanov, 2014, Volatiles in lunar regolith samples: A survey. Sol. Syst. Res. 48, 113–129.

4: Mateo et al., 2019, Lanzarote and Chinijo Islands Geopark:From Earth to Space. Springer International Publishing.

How to cite: Melchiori, G., Massironi, M., Pozzobon, R., Ferretti, P., and Calvari, S.: Unravelling similarities between Mount Etna's pyroclastic deposits and the Lunar counterparts., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17694, https://doi.org/10.5194/egusphere-egu25-17694, 2025.

EGU25-18054 | ECS | Orals | PS7.5

Modelling surface mineral diversity of atmosphere-free rocky exoplanets for spectroscopic characterisation 

Rob Spaargaren, Antonio Manjon Cabeza Cordoba, Maxim Ballmer, and Tim Lichtenberg

Observations of several short-period rocky exoplanets (e.g., LHS 3844 b, TRAPPIST-1 b, GJ 367 b) suggest that they do no host substantial secondary atmospheres, which makes their surfaces directly accessible to spectral characterisation. Various minerals and rock types have potentially distinguishable surface reflectance spectra, allowing for observational characterisation of surface geology for such atmosphere-less exoplanets. While extensive surface spectra for Solar System lithologies are available, they may not capture the full range of surface diversity, as rocky exoplanets display a bulk compositional diversity far exceeding that seen in the Solar System. To address this gap, we explore potential surface mineralogies of volatile-free rocky exoplanets, with compositional diversity informed by stellar abundances.
 
We model magma compositions formed from bulk mantle melting in the NCFMASCr system with a Gibbs free energy minimization algorithm, Perple_X. Bulk mantle compositions are systematically varied in terms of relative abundances of Mg, Si, Ca, Al, and Na, informed by stellar abundances, while keeping Fe and Cr constant and equal to the Earth bulk mantle. We then use the same modelling set-up to derive crustal mineralogy for bulk crust compositions based on these magmas. 
 
Surface mineralogy primarily varies with the bulk mantle Mg/Si ratio: Si-rich mantles produce quartz- and plagioclase-dominated crusts, intermediate planets produce pyroxene- and plagioclase-dominated crusts, and Mg-rich planets produce crusts consisting of olivine, spinel, and nepheline. Increasing the abundances of Ca, Al, and Na mainly results in a widening of the clinopyroxene, spinel, and nepheline stability fields. The crusts of Mg-rich planets are experimentally under-explored, while we predict a significant fraction of all rocky exoplanets to form such crusts. Thus, additional surface reflectance spectra measurements are required to fully cover the diversity of potential rocky exoplanet surfaces and to enable accurate interpretation of future observations of their surface geology.

We further show with geodynamical simulations that the high-pressure density contrast between crustal and mantle rocks plays a first-order role in thermal and dynamical evolution of rocky exoplanet interiors. Planets with a greater density contrast tend to stabilize a layered mantle structure, where subducted crust accumulates at the bottom of the mantle, overlain by a cold, depleted, and typically ultramafic upper mantle. Calculating the density contrast between crust and mantle rocks for our sample of exoplanet compositions at a pressure of 140 GPa, we find that most Mg-rich planets form crusts that are significantly denser than the residual mantle, forming such a double-layered mantle structure. Meanwhile, the most Si-rich mantles produce granite-like crusts, which we predict to be too buoyant to subduct. Only planets with intermediate Mg/Si, which includes the solar system planets, have crustal buoyancy that allows for subduction and mixing of subducted crust with the mantle on geological timescales. Thus, constraining rocky exoplanet crust mineralogy and density is essential for understanding their long-term evolution and for interpreting spectroscopic observations of such planets, which is possible with JWST.

How to cite: Spaargaren, R., Manjon Cabeza Cordoba, A., Ballmer, M., and Lichtenberg, T.: Modelling surface mineral diversity of atmosphere-free rocky exoplanets for spectroscopic characterisation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18054, https://doi.org/10.5194/egusphere-egu25-18054, 2025.

EGU25-19233 | ECS | Posters on site | PS7.5

Photometric-Constrained Reconstruction of Lunar Landing Site Topography Using Orbiter and Descent Images 

Xiaohuan Xie, Shijie Liu, Li Ma, Qian Huang, Hao Chen, Jürgen Oberst, and Xiaohua Tong

In lunar exploration, high-resolution topography is an important basis for safe landing and mission planning. Remote sensing images are the main data sources for the reconstruction of lunar surface topography [1]. Among them, the orbiter images preserve the topographic photometric information under different illumination directions, and the descent images contain high-resolution morphological details of the landing site. In order to integrate the advantages of multi-illumination directions of orbiter images and high resolution of descent images, we propose a joint photometric-constrained method for topography reconstruction using both orbiter and descent images. In the framework of the joint photometric-constrained Shape from Shading (SfS) [2-4], the photometric information in multi-source images illuminated from different directions is added into the cost function as a weighted regular term in topography reconstruction. We focus on the Chang'E-3 landing site. We used the Lunar Reconnaissance Orbiter (LRO) Narrow Angle Camera (NAC) images of the area and Chang'E-3 descent images for experiments, and obtained topographic data of the site with a resolution better than 0.1 m/pixel. Comparing with previously derived topography [5], we verified that our topography is more consistent result with the images in multi-angle illumination rendering [6], integrating the photometric information of the multi-source images and preserving the morphological details such as small-size impact craters. The method proposed in this study not only improves the accuracy of topography reconstruction of the Chang'E-3 landing site, but also provides a new idea for the joint processing of multi-source image data.

[1] Di K., et al. (2020) Topographic mapping of the moon in the 21st century: from hectometer to millimeter scales. The International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, XLIII-B3-2020, pp.1117-1124.

[2] Horn, B.K.P. (1990) Height and gradient from shading. International Journal of Computer Vision, 5, pp. 37–75.

[3] Beyer R.A., et al. (2018) The Ames Stereo Pipeline: NASA's Open Source Software for Deriving and Processing Terrain Data. Earth and Space Science, 5, pp. 537-548.

[4] Tenthoff M. et al. (2020) High Resolution Digital Terrain Models of Mercury. Remote Sensing, 12, p. 3989.

[5] Henriksen M.R., et al. (2017) Extracting accurate and precise topography from LROC narrow angle camera stereo observations. Icarus, 283, pp.122-137.

[6] Tong X., et al. (2023) A high-precision horizon-based illumination modeling method for the lunar surface using pyramidal LOLA data. Icarus, 390, p. 115302.

How to cite: Xie, X., Liu, S., Ma, L., Huang, Q., Chen, H., Oberst, J., and Tong, X.: Photometric-Constrained Reconstruction of Lunar Landing Site Topography Using Orbiter and Descent Images, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19233, https://doi.org/10.5194/egusphere-egu25-19233, 2025.

EGU25-19374 | ECS | Posters on site | PS7.5 | Highlight

Microorganisms under simulated icy moon environments project (micro icy) : a step foward to solar system exploration 

Alessia Cassaro, Claudia Pacelli, Lorenzo Cocola, Angelina Cordone, Marta Del Bianco, Mattia Esposito, Francesca Ferranti, Lorenzo Manfrin, Luca Parca, and Angelo Zinzi

Astrobiological research aims to find evidence of life in the Solar System's habitable environments, prioritizing icy moons with potential subsurface oceans (Lunine, 2017).  Subsurface liquid water is evidenced on Europa, Ganymede, Callisto (Kivelson et al., 2000), and Enceladus (Spencer & Nimmo, 2013). Enceladus, studied via Cassini’s remote sensing, is of particular interest due to its active surface and global subsurface salty ocean (Thomas et al., 2016; Postberg et al., 2009). Jets of icy particles and water vapor observed at its south pole (Porco et al., 2006) suggest a subsurface aquifer with potential for life (Fuller et al., 2016; Porco et al., 2017; Lainey et al., 2018).

To explore habitability, remote sensing relies on understanding life in Earth’s extreme environments, such as hydrothermal systems, where microbial communities thrive under harsh conditions. The Strytan shallow-water hydrothermal vents in Iceland serve as an ideal analogue for icy moons, as they mimic similar geological processes. In this context, the MICRO ICY project aims to study microbial life in these environments to identify potential biosignatures and better understand microbial adaptation to extreme conditions, advancing life-detection missions.

The project will aim to (i) sampling fluid samples from Strytan shallow-water hydrothermal vents in Iceland, (ii) identifying the cultivable microbial portion, (iii) studying the whole microbial communities through metabarcoding identification and its adaptaption mechanisms by applying -omics approaches, (iv) identifying functionality and genomic traits of interest for adaptation and resistance to extreme conditions by metagenomic approach. In addition, gas composition signatures related to the activity of microbes will be investigate, by using mass spectrometry.

 

The MICRO ICY project aims to achieve the following results:

- a proof of concept for using the Strytan shallow-water hydrothermal vents in Iceland as analogues for the subsurface environments of icy moons;

- define the habitats and assess criteria for habitability on icy moons through a complete characterization of geo-microbial context of the Strytan shallow-water hydrothermal vents, including the evaluation of microorganism biodiversity and functionality;

-  identify the adaptation strategies of selected microbes to simulated planetary environments through transcriptomic and proteomic approaches;

- improve our knowledge of the behaviour of terrestrial extremophiles to planetary analogue environments as support for the search for life beyond Earth;

- identify the gas signatures of microbial life in simulated planetary environments with spectrometry analyses;

Here, we reported preliminary results from geochemical analyses of the Strytan shallow-water hydrothermal vent samples, performed by using Inductively Coupled Plasma Mass Spectrometry (ICP-MS) and Ion Chromatography (IC). Concurrently, ongoing experiments involving both culture-dependent (extremophilic microorganism isolation) and culture-independent (metagenomics) approaches aim to identify the most suitable organisms for exposure in an Enceladus simulation chamber, to assess their ability to grow and survive in extraterrestrial environments.

How to cite: Cassaro, A., Pacelli, C., Cocola, L., Cordone, A., Del Bianco, M., Esposito, M., Ferranti, F., Manfrin, L., Parca, L., and Zinzi, A.: Microorganisms under simulated icy moon environments project (micro icy) : a step foward to solar system exploration, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19374, https://doi.org/10.5194/egusphere-egu25-19374, 2025.

EGU25-19657 | ECS | Posters on site | PS7.5

High-resolution Illumination Maps around the Lunar South Pole 

Qian Huang, Shijie Liu, Hao Chen, Philipp Gläser, Fan He, Jürgen Oberst, and Xiaohua Tong

With the Moon’s rotation axis almost perpendicular to the ecliptic, the lunar polar regions are in a unique position. As the Sun hovers near the horizon all year round, and given the rough morphology, this leads to very complex illumination conditions in the area. High-resolution illumination maps derived from accurate lunar terrains serve as essential tools for identifying cold traps and evaluating solar energy ― key factors for upcoming exploration missions [1], [2]. Here, we use our previously developed illumination modeling methodology [3] to produce a series of illumination maps based on Lunar Orbiter Laser Altimeter (LOLA) gridded topographic models. Benefitting from the methodological optimizations and GPU acceleration techniques, modeling efficiency is no longer a challenge. We produced maps of the average illumination and the distribution of Permanently Shadowed Regions (PSRs), the resolution and coverage of these maps are consistent with the LOLA terrains, up to a maximum resolution of 5 meters [4]. Another derivative of modeling, the artificially shaded synthetic images corresponding to illumination at any moment, can be compared with “real” image data. We selected Malapert Massif and Shackleton-de Gerlache Ridge (both near the candidate landing sites of the Artemis program) as our experimental areas, and compared our maps with previously published illumination data [1], [2]. The results show that, our higher-resolution illumination maps are visibly more informative and the corresponding synthetic images are more consistent with the illumination patterns seen in “real” images. This work can provide useful suggestions for future lunar south pole explorations and scientific research.

 

[1] Mazarico E., et al. (2011) Illumination conditions of the lunar polar regions using LOLA topography. Icarus, 211, pp.106681.

[2] Gläser, P., et al. (2018) Illumination conditions at the lunar poles: Implications for future exploration. Planetary and Space Science, 162, pp.170-178.

[3] Tong, XH., et al. (2022) A high-precision horizon-based illumination modeling method for the lunar surface using pyramidal LOLA data. Icarus, 390, pp.115302.

[4] Barker et al. (2023) A New View of the Lunar South Pole from the Lunar Orbiter Laser Altimeter (LOLA). The Planetary Science Journal, 4, pp.183.

How to cite: Huang, Q., Liu, S., Chen, H., Gläser, P., He, F., Oberst, J., and Tong, X.: High-resolution Illumination Maps around the Lunar South Pole, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19657, https://doi.org/10.5194/egusphere-egu25-19657, 2025.

EGU25-19966 | Orals | PS7.5

Updates to the TGO-CaSSIS Stereo Products Generation and the INAF public catalog of DTMs 

Adriano Tullo, Cristina Re, Emanuele Simioni, Silvia Bertoli, Riccardo La Grassa, Gabriele Cremonese, and Nicolas Thomas

In orbit since the April 2018, the Colour and Stereo Surface Imaging System (CaSSIS) on board of the ExoMars Trace Gas Orbiter (TGO) has recently entered its 6th year of scientific phase. Since then, CaSSIS has provided us with a rich catalog of up to four bands stereo images of the Martian surface. The stereo capability is achieved through an innovative telescope rotation approach composing a convergence angle of almost 22 degrees between the stereo couple. In this way CaSSIS can produce detailed color 3D maps, thus providing crucial data for the analysis of the surfaces and their composition.

The pipeline for three-dimensional modelling is developed and maintained by the INAF team located at the Astronomical Observatory of Padova, making available the Digital Terrain Models (DTMs) and orthorectified images to the entire team and scientific community since the start of the mission.

The 3DPD software (Simioni et al., 2021; Re et al., 2022), at the core of the pipeline, allows the exploitation of data according to the principles of stereogrammetry. The DTMs are produced at 13.5 m ground sample distance from 4.5 m/px images, with an estimated vertical accuracy below 3 pixels size (15 m)  (Fig.1).

To date, more than 2100 stereo couples are available on a total of 40.000 images acquired. Of these about 400 stereo pairs have already been processed and available for download at  the OAPD-hosted repository (https://cassis.oapd.inaf.it/archive/).

Since the framework was first founded by Simioni et al., 2021, the pipeline has been continuously developing to improve the performance of the data product generation.

The goal of this work is to present the actual state of the framework and all the improvements made. Recent changes are here described and supported by an assessment of the quality and precision of the generated products and their derivatives.

Recent developments include the integration of the Bundle Block Adjustment, employing the jigsaw routines made available with the USGS ISIS platform (Laura et al., 2023). Thanks to the jigsaw output, we are able to refine the projection matrices affected otherwise by distortions that introduce geometric effects of misalignments between the acquisitions. The misalignments not adequately modelled and resolved by the Bundle Adjustment could otherwise result in steps artefacts that can reach even hundreds of m in the worst cases.

Further important update is given by an innovative approach of aligning DTMs to MOLA-HRSC (Fergason et al., 2018), further improving the surface projection and the absolute elevation, reaching values generally below 50 m/px of standard deviation in comparison with it. This process was also extended to the entire database of DTMs already produced as one major update, bringing similar results (Fig.2).

Fig.1 Comparison between a CaSSIS DTM (MY34_003673_018) and a HiRISE DTM (DTEEC_005533_1975_005388_1975) at 1 m/px, demonstrating a vertical accuracy of about 8m.

 

Fig.2 The standard deviation on the vertical accuracy, achieved as a result of the recent alignment with the MOLA-HRSC and applied to the entire CaSSIS DTMs database.

How to cite: Tullo, A., Re, C., Simioni, E., Bertoli, S., La Grassa, R., Cremonese, G., and Thomas, N.: Updates to the TGO-CaSSIS Stereo Products Generation and the INAF public catalog of DTMs, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19966, https://doi.org/10.5194/egusphere-egu25-19966, 2025.

EGU25-20078 | ECS | Posters on site | PS7.5

Categorization of ring and bulge topographies of infilled craters on Mercury 

Gene Schmidt, Salvatore Buoninfante, Valentina Galluzzi, and Pasquale Palumbo

Mercury boasts a variety of infilled craters, several of which contain central depressions surrounded by unique, bulged, ring-like structures. These rings are comprised of the infill itself, range in size and elevation, and can often exceed the crater rim in which they are contained (e.g. Bryne et al., 2014). Although peak ring crater types are common across Mercury (e.g. Baker et al., 2011; Schon et al., 2011), these bulged infill rings represent an entirely different morphology which represents a process that occurs after the crater and potential peak ring is formed. These bulged rings often present concentric extensional faults on their summits, and in some cases the accompanying central depression contains radial or circular extensional faults (e.g. Cunje & Ghent, 2016; Marchi et al., 2011). The formation process of this topography remains unknown and difficult to constrain, however it has been previously suggested that global contraction could aid their formation (Byrne et al., 2014). However, the weight load of the infill itself has yet to be fully appreciated as a candidate for tectonic processes on Mercury, particularly in the creation of bulged topography (Schmidt & Salvini, 2024). Additionally, lava entry pathways (i.e. lava which exploits circular normal faults within the interior of the craters) may play a role. By analyzing nine craters (four exhibiting the bulged infill topography, four exhibiting peak ring topography, and one seemingly intermediate type of topography) we aim to determine the relationship between bulged rings within infill and their more common peak ring topography counterparts. In so doing, we can determine if this infill topography is merely a lava infill which has conformed to a pre-existing peak ring, or if the weight load of the infill at the center of the crater has the potential to create an elastic response which creates the bulged ring and simultaneously the central depression.

We gratefully acknowledge funding from the Italian Space Agency (ASI) under ASI-INAF agreement 2024-18-HH.0

Baker et al. (2011) The transition from complex crater to peak-ring basin on Mercury: New observations from MESSENGER flyby data and constraints on basin formation models. Planetary and Space Science, 59(15), 1932-1948.

Byrne et al. (2014) Mercury’s global contraction much greater than earlier estimates. Nature Geoscience, 7(4), 301-307.

Cunje & Ghent (2016) Caloris basin, Mercury: History of deformation from an analysis of tectonic landforms. Icarus, 268, 131-144.

Marchi et al. (2011) The effects of the target material properties and layering on the crater chronology: The case of Raditladi and Rachmaninoff basins on Mercury. Planetary and Space Science, 59(15), 1968-1980.

Schmidt & Salvini (2024) Thickness of Pluto's Ice Shell from elastic deformation of the Sputnik Planitia forebulge: Response to infill load or vestige of impact event?. Earth and Planetary Science Letters, 646, 118974.

Schon et al. (2011) Eminescu impact structure: Insight into the transition from complex crater to peak-ring basin on Mercury. Planetary and Space Science, 59(15), 1949-1959.

How to cite: Schmidt, G., Buoninfante, S., Galluzzi, V., and Palumbo, P.: Categorization of ring and bulge topographies of infilled craters on Mercury, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20078, https://doi.org/10.5194/egusphere-egu25-20078, 2025.

Soil moisture (SM) is a relatively active surface parameters that are significant to the sustainable development of the water–land–air–plant–human nexus. In response to the requirements of multiscale product validation and multisource uncertainty tracking, a soil moisture monitoring network in the Qinghai Lake Basin (QLB-NET) was established in September 2019. The QLB-NET is characterized by densely distributed in situ sites (82 sites) measuring SM and ST at 5-, 10-, and 30-cm depths, with 60 sites in a large-scale network in a heterogeneous area of 36 km × 40 km, which covers the SMAP, AMSR2, SMOS pixel footprint, and 22 sites evenly distributed across two small-scale 1 km × 1 km networks for sub-grid analysis. The site deployment strategy, the installation and maintenance, the sensor calibration, and the characteristics and quality of the in situ SM measurements of QLB-NET will be introduced in detail. Quantitative analyses of the in situ measurements was carried out, which shows that the QLB-NET can provide stable and reliable ground truth for SM over coarse grid scales, facilitating product validation and uncertainty tracking, spatiotemporal analysis of SM change optimization of the SM retrieving algorithms and scaling methods in heterogeneous regions.

How to cite: Zhu, Z.: The Dataset of Dense Soil Moisture Monitoring Network in the Qinghai Lake Basin on the Qinghai–Tibetan Plateau, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1605, https://doi.org/10.5194/egusphere-egu25-1605, 2025.

EGU25-11764 | Posters on site | HS8.3.2

Integration of soil moisture measurements into the observation network of the German Meteorological Service – the project IsaBoM 

Wolfgang Kurtz, Mario Albert, Mathias Herbst, Leonhard Hufnagl, and Jan Lenkeit

As many other European countries, Germany has been affected by an increasing number of both drought and flood events in the last couple of years that had considerable negative impacts on the agricultural and forestry sector. These events led to an increasing information demand of stakeholders, practitioners and the general public on critical variables such as soil moisture.  Area-wide information on soil moisture is most often derived indirectly from hydrological model simulations, one of them being DWD’s soil moisture viewer which is based on the soil-vegetation-atmosphere-model AMBAV. Besides model-based soil moisture information, which is strongly influenced by model assumptions and parameterisation, a number of institutions started to build-up local soil moisture observation networks, such as the TERENO network, that also provide in-situ observations of soil moisture states. However, a nationwide observation network for (standardised) soil moisture observations is still lacking in Germany.

The project IsaBoM (“Integration of standardised and automatized soil moisture measurements in the DWD observation network”), an internal project of the German Meteorological Service (DWD), strives to establish the technical and scientific basis for introducing standardised soil moisture observations in DWD’s operational meteorological observation network. This includes e.g. the choice of suitable sensors and measurement protocols, calibration procedures for selected sensors, quality-control measures and establishing data flow and automated data provisioning. The final goal is to equip about 25 stations throughout Germany with cosmic-ray neutron sensing (CRNS)-devices and in-situ profile measurements of soil moisture where the chosen locations should provide a representative subset in terms of soil properties and climatic conditions. Here we present the overall network design as well as first comparisons between soil moisture data obtained by different CRNS-sensors at two sites that have a broad range of complementary agrometeorological measurements in place that facilitate a thorough interpretation of the results.

How to cite: Kurtz, W., Albert, M., Herbst, M., Hufnagl, L., and Lenkeit, J.: Integration of soil moisture measurements into the observation network of the German Meteorological Service – the project IsaBoM, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11764, https://doi.org/10.5194/egusphere-egu25-11764, 2025.

EGU25-13338 | Posters on site | HS8.3.2

Enhancing Soil Moisture Prediction with Data-Driven Models: A Global Perspective 

Steven Hristopoulos, Gabriel Moraga, and Noah Pearson Kramer

The prediction of soil moisture plays a vital role in assessing water availability, optimizing agricultural resources, and preparing for climate-induced disasters. However, significant gaps remain in soil moisture observation networks due to data sparsity, inconsistent temporal coverage, and limited spatial resolution, particularly in underrepresented regions. The International Soil Moisture Network (ISMN), the largest archive of in situ soil moisture data, highlights these challenges, with many datasets averaging only a decade of temporal coverage and biased spatial distribution heavily skewed toward the Global North. This study presents a data-driven modeling framework designed to enhance soil moisture prediction by leveraging advanced machine learning techniques, diverse geospatial datasets, and in situ observations.

Our multi-stream model integrates high-resolution data from Sentinel-2 (NDVI, B4, B8), ECMWF weather forecasts, and SRTM elevation models to predict surface and rootzone soil moisture at six-hour intervals. Validation against SMAP L4 datasets demonstrates high accuracy, achieving mean RMSE values of 0.1087 m³/m³ for surface moisture and 0.1183 m³/m³ for rootzone moisture across 20 Köppen-Geiger climate zones. The modular design enables the model to adapt to diverse climatic conditions and refine predictions through continuous validation. Performance analysis reveals strong temporal generalization and superior results in wet climates, though arid and extreme environments pose challenges, highlighting areas for targeted improvements.

To address data sparsity, the study emphasizes balanced sampling and the integration of citizen science initiatives, which supplement traditional networks by providing localized, high-frequency observations. By incorporating in situ ISMN datasets, the framework aligns with the session's focus on improving observation networks and leveraging data quality assurance. Additionally, hybrid approaches that combine physical constraints with machine learning models ensure predictions are grounded in realistic soil behavior and spatial consistency.

This research underscores the importance of sustained investment in developing and maintaining soil moisture observation networks, particularly in underrepresented regions. It highlights the need for standardized data collection protocols, advanced calibration techniques, and open-access platforms that integrate in situ and satellite observations. By bridging gaps in traditional networks, the model advances global soil moisture monitoring, supporting applications in sustainable agriculture, water resource planning, and climate resilience.

Aligned with session HS8.3.2, this study exemplifies the role of innovative measurement techniques and data-driven approaches in enhancing the utility of soil moisture datasets. The findings advocate for a collaborative scientific effort to address the pressing challenges of data availability, quality assurance, and network deployment. Through scalable modeling frameworks, this research sets the foundation for predictive systems that provide actionable insights to policymakers and practitioners in hydrology, agriculture, and climate science.

How to cite: Hristopoulos, S., Moraga, G., and Pearson Kramer, N.: Enhancing Soil Moisture Prediction with Data-Driven Models: A Global Perspective, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13338, https://doi.org/10.5194/egusphere-egu25-13338, 2025.

EGU25-13801 | Posters on site | HS8.3.2

How well do gridded products represent soil moisture signatures in natural ecosystems during precipitation events? 

Mauricio Zambrano-Bigiarini, Daniel Nuñez-Ibarra, and Mauricio Galleguillos

Soil moisture (SM) is a key factor influencing the interactions between the atmosphere and processes at the Earth’s surface. Recent advances in remote sensing and land surface modelling have improved the estimation of soil moisture in ungauged areas.

This study evaluates the performance of four state-of-the-art gridded SM products - SPL4SMAU, GLDAS, ERA5 and ERA5-Land - compared to in situ measurements at ten sites located in near-natural shrublanbd and native forest ecosystems of the semi-arid and humid regions of central and southern Chile (five in the semi-arid north and five in the humid south). The unbiased root mean square error (ubRMSE), Pearson’s product-moment correlation coefficient (r) and modified Kling-Gupta efficiency (KGE') were used as performance metrics to evaluate the representation of surface soil moisture (SSM) and root zone soil moisture (RZSM). In addition, event rising time (RT) and amplitude (A) were used as SM signatures to assess the dynamic aspects of the soil moisture time series and to enable process-based model evaluations.

Our results show that SPL4SMAU achieves the lowest ubRMSE for both SSM and RZSM, especially in the northern region. However, ERA5 and ERA5-Land outperformed SPL4SMAU in terms of linear correlation and KGE', with particularly good results in the humid south. In terms of SM responses to the first precipitation event of the year, SSM amplitude was generally higher in the humid south, with SPL4SMAU and ERA5-Land very close to in situ values, while GLDAS showed a lower sensitivity to precipitation. As expected, all datasets showed a slower response for RZSM compared to SSM, with GLDAS showing the longest rising times in both regions. On the other hand, SPL4SMAU and GLDAS showed a stronger increase in SSM amplitude in the south for the most intense precipitation event of the year, while ERA5-Land showed more moderate rising times, which is consistent with the in-situ data.

Overall, ERA5-Land and ERA5 proved to be reliable datasets for representing the spatio-temporal variability of SM in central and southern Chile, especially in the southern ecosystems, while SPL4SMAU performed well in terms of uRMSE but showed large variability in the other metrics analysed.

We gratefully acknowledge the financial support of ANID-Fondecyt Regular 1212071, 1210932, ANID-PCI NSFC 190018, and ANID/FONDAP 1523A0002.

How to cite: Zambrano-Bigiarini, M., Nuñez-Ibarra, D., and Galleguillos, M.: How well do gridded products represent soil moisture signatures in natural ecosystems during precipitation events?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13801, https://doi.org/10.5194/egusphere-egu25-13801, 2025.

EGU25-15016 | ECS | Posters on site | HS8.3.2

Monitoring deep unsaturated zones in Western Australia to reveal crucial insights for water resources management 

Simone Gelsinari, Sarah Bourke, Richard Silberstein, and Sally Thompson

Soil moisture observations have been collected since the late 1950s and are relatively abundant in the northern hemisphere. These readings are generally taken at shallow depths with sensors rarely installed more than 2 metres below the surface. However, deep soil moisture dynamics can play a crucial role in determining ecosystem services, land-atmosphere water fluxes, plant water use, nutrient cycle and, eventually, groundwater recharge. In thick unsaturated zones, shallow soil moisture observations are likely to fail to capture important hydrological processes, and their feedback with the atmosphere, generating significant uncertainties. 

Here we present the results from a soil moisture monitoring network established as part of the Recharge in a Changing Climate (RiCC) project. The network aims to capture soil moisture dynamics in deep sandy profiles of a Mediterranean-like zone in Western Australia, where traditional shallow and surface soil moisture observations fall short of detecting significant hydrological processes. The monitoring network, deployed since 2022, comprises over 75 sensors strategically distributed across 7 locations over the Swan Coastal Plain at depths of up to 9 m to provide continuous high-frequency soil moisture data. These soil moisture sensors are complemented by 14 access tubes where neutron moisture probe readings are taken to characterize the spatial heterogeneity.

Findings reveal complex patterns of moisture movement through the profile, with significant temporal variations in wetting front depths and propagation patterns, improving the representation of soil water/vegetation interaction, and providing unique insights into groundwater recharge processes in sandy aquifer systems. These observations challenge existing assumptions about soil water movement in sandy soils and provide crucial validation data for improving ecohydrological models and recharge quantification. Information from the RiCC monitoring campaign can significantly reduce uncertainties in water resources management and, by including transpiration from deeper soil moisture pools, enhance the accuracy of modelled land-atmosphere feedback. These insights are also beneficial for understanding the resilience of ecosystems and agroecosystems under transient climate conditions.

How to cite: Gelsinari, S., Bourke, S., Silberstein, R., and Thompson, S.: Monitoring deep unsaturated zones in Western Australia to reveal crucial insights for water resources management, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15016, https://doi.org/10.5194/egusphere-egu25-15016, 2025.

EGU25-15693 | ECS | Posters on site | HS8.3.2

Drone-based multiband Synthetic Aperture Radar (UAV-RADAR) for soil moisture assessment 

Daniel Evans, Bernardo Candido, and Armando Marino

Soil moisture plays a vital role in agriculture, drought management, and flood prevention. It is essential for plant growth and sustainable farming practices. In flood-prone areas, soil's ability to retain water helps absorb excess moisture and reduce runoff, mitigating flood risks. Therefore, effective soil moisture monitoring is crucial for informed irrigation and water management decisions. Various methods exist for measuring soil moisture, both in-situ and remote. In-situ techniques, like volumetric and gravimetric sampling, provide real-time data but are limited to specific locations unless interpolation is applied. On the other hand, remote sensing offers broader spatial coverage but often with lower resolution and accuracy. While remote sensing can validate ground-based data, it is less effective for capturing short-term changes, such as those resulting from irrigation, at fine temporal scales.

To address these challenges, we are developing UAV-RADAR, the first multiband Synthetic Aperture Radar (SAR) mounted on a drone. Unlike conventional SAR platforms (e.g., Sentinel-1), UAV-RADAR provides rapid, high-resolution, and scalable soil moisture data tailored to specific agricultural and environmental contexts. Its customizable flight plans enable detailed pre- and post-treatment analyses, capturing temporal changes with unprecedented flexibility.

In this presentation, we will showcase our current research and development of UAV-RADAR to date, demonstrating its capability to measure soil moisture across diverse soil types, landscapes, and agricultural practices. Using data from proof-of-concept experiments carried out in England and Wales, we will show soil moisture maps and demonstrate their applications. We will highlight use cases, and explore how UAV-RADAR can contribute to initiatives like the International Soil Moisture Network.

How to cite: Evans, D., Candido, B., and Marino, A.: Drone-based multiband Synthetic Aperture Radar (UAV-RADAR) for soil moisture assessment, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15693, https://doi.org/10.5194/egusphere-egu25-15693, 2025.

The Network of stations for the Monitoring of physical Parameters of Soils in Catalonia (XMS-Cat) acquires and provides continuous data on in situ soil temperature and moisture at different depths of the soil profile. Initiated in 2015, this relatively young network currently comprises 19 stations and is expanding at a steady rate of two stations per year, aiming for full coverage of the region. Accelerated coverage expansion is planned through data-hosting agreements with privately owned stations, such as those associated with wine protected designations.
The network has recently undertaken a comprehensive review and assessment of its deployment, installation, and data quality assurance protocols to ensure adherence to established best practices, long-term viability, and consistency with other networks.
This contribution provides an overview of the XMS-Cat network and presents the preliminary results of the ongoing review. The aim is to foster dialogue among networks and stakeholders while leveraging the collective knowledge of this dynamic community.

How to cite: Portell, X., Boquera, L., Vicens, M., and Lladós, A.: Review and assessment of current protocols of the Network of stations for the Monitoring of Physical Parameters of Soils in Catalonia (XMS-Cat), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15705, https://doi.org/10.5194/egusphere-egu25-15705, 2025.

EGU25-15709 | Posters on site | HS8.3.2

Cosmic Rays Neutron Sensing for soil moisture monitoring in vineyard with variable soil conditions 

Marcella Biddoccu, Gazzola Enrico, Giorgio Capello, Davide Gisolo, Stefano Gianessi, Stefano Bechis, and Stefano Ferraris

Cosmic Rays Neutron Sensing (CRNS) is a well-known method in Hydrology that allows to measure soil water content on a large scale and in depth. It is based on the detection of cosmogenic neutrons, particles generated by the interaction of cosmic rays with the atmosphere, after their interaction with the soil where they can be effectively absorbed by water molecules. The signal collected by a single CRNS probe in terms of neutron count rate is sensitive to soil moisture within a volume spanning up to a dozen hectares and up to 50 cm depth, in real-time, positioning itself in a horizontal spatial scale in between point measurements and satellites.

In order to evaluate the effectiveness of CRNS to give information about soil moisture in an agricultural system with different soil conditions, a site in the Alto Monferrato vine-growing area (Piedmont, NW Italy) was equipped with a Finapp CRNS probe since August 2023. The site has two vineyard-field-scale plots with inter-rows managed with conventional tillage (CT) and grass cover (GC), respectively. More than 20 sensors are located in different positions and depths (from 10 to 50 cm) in the vineyard, including the STEMS network that is part of the International Soil Moisture Network. Precipitation measurements on site are available over more than 20 years, show that 2023 was very dry, with Standardized Precipitation Index lower than -1 for most of the year, whereas 2024 was increasingly wet, with exception of first two months of the year.

Available soil moisture data from CRNS and sensors have been compared until autumn 2024, using statistical indexes such as the efficiency coefficient of Nash and Sutcliffe (NSE), root mean square error of residuals (RMSE) and the coefficient of determination of the linear regression (R2). The analysis was carried out separately for the two years, which were considered respectively dry and wet.

Statistics showed that in the last 5 months of 2023 (dry period) there was a good agreement of soil moisture values measured by sensors between 10 and 20 cm of depth with both soil management, with different results according to the position, the best reported in the middle of the GC inter-row at depth of 20 cm (R2=0.913, NSE=0.756, RMSE=0.25). The results for 2024, which was a wetter year, showed great variability, such as the values recorded by the sensors, with unsatisfactory statistics, since best values for indexes were obtained for the sensor placed in the middle of CT inter-row (R2=0.598, NSE=0.485, RMSE=0.118).

Thus, in the dry period the CRNS probe gave good information on soil moisture conditions in the most superficial layer disregarding the soil management of the vineyard. On the contrary, the difficulty in having good agreement in wet conditions can be due to the high spatial variability of soil moisture both in the horizontal and in-depth directions, soil saturation and ponding, in addition to variable conditions of soil conditions (i.e. soil density) depending to soil management and tractor traffic during the growing season.

How to cite: Biddoccu, M., Enrico, G., Capello, G., Gisolo, D., Gianessi, S., Bechis, S., and Ferraris, S.: Cosmic Rays Neutron Sensing for soil moisture monitoring in vineyard with variable soil conditions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15709, https://doi.org/10.5194/egusphere-egu25-15709, 2025.

Surface soil moisture (SSM) plays a significant role in the energy exchanges and the complex interaction within the air–soil–water–plant-human nexus. To better evaluate and utilize the microwave remote sensing (RS) SSM products at coarse scale (e.g., 0.25°) and the retrieved SSM data at fine-scale (e.g., 1 km), a pixel-scale reference dataset should be generated within the area of in-situ network. However, in the Tibetan Plateau (TP), where in-situ SSM data is sparse and limited, the current fine-scale SSM datasets generated using machine learning (ML) methods face certain limitations in terms of spatial extrapolation capability. In this study, we developed a framework that integrated ML method with geostatistical spatiotemporal fusion method to generate long-term and seamless 1 km SSM dataset with higher spatial extrapolation accuracy. The study area included five ground observation network regions (Shiquanhe, Pali, Naqu, Heihe and Maqu). Firstly, the incomplete 1 km scale SSM was retrieved by upscaling the in-situ SSM using the Residual Dense Network (RDN) model. Then, the Bayesian maximum entropy (BME) method, considering the uncertainties of the upscaled SSM, was employed to spatiotemporally fuse upscaled and in-situ SSM to improve the accuracy of spatial extrapolation. Validation based test sites shows that the accuracy of the fused SSM data was improved across all five regions, with the improvement in ubRMSE ranging from 3.33% to 21.28%, resulting in an overall increase of 8.2%. The fused SSM can more effectively capture the temporal variability of the measurements of test stations. The results demonstrate that the proposed framework effectively generates a reference SSM dataset within the ground observation network area.

How to cite: Zhu, Z.: Generation of long-term and seamless 1 km surface soil moisture dataset within the area of in-situ network, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18617, https://doi.org/10.5194/egusphere-egu25-18617, 2025.

EGU25-1197 | PICO | CR6.2

Airborne radar polarimetry over the Northeast Greenland Ice Stream 

Olaf Eisen, Daniela Jansen, Steven Franke, Veit Helm, Ole Zeising, Charlotte Carter, Tamara Gerber, Niels Nymand, Dorthe Dahl-Jensen, John Paden, and Daniel Steinhage

Ice streams are important export routes for ice from the interior of ice sheets to the ocean and a key component for projecting future sea level rise under continued climate heating. Over the last years, evidence emerged that the distribution of ice crystals in and near ice streams is highly anisotropic and strongly influences the viscosity of the ice. To map this crystal orientation fabric (COF) in space, radio-echo sounding has been proven as the most effective way. Several methods to deduce COF were applied to co-polarized airborne and ground-based radar data (i.e. all antennas have the same polarization direction) and tied to ice cores, with extensive coverage available around the EastGRIP ice core to analyse the COF within the Northeast Greenland Ice Stream (NEGIS). We extended this application to a new setup of cross-polarimetric surveys with AWI's ultrawideband airborne radar system and performed several surveys over NEGIS in 2022. 
Our presentation focuses on the results of this survey obtained from established methods to obtain the COF and compares them to ground-based results, such as from phase-sensitive radio-echo sounding (pRES) and a ground-based polarimetric radar system. We discuss the advantages of operating airborne radar systems in a cross-polarized mode in contrast to only co-polarized configurations to provide insights into fabric distribution on larger spatial scales as well as the disadvantages from a lower signal-to-noise ratio for imaging the bed as well as sounding internal layers.

How to cite: Eisen, O., Jansen, D., Franke, S., Helm, V., Zeising, O., Carter, C., Gerber, T., Nymand, N., Dahl-Jensen, D., Paden, J., and Steinhage, D.: Airborne radar polarimetry over the Northeast Greenland Ice Stream, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1197, https://doi.org/10.5194/egusphere-egu25-1197, 2025.

EGU25-1493 | PICO | CR6.2

Surface melt driven changes to ice properties for a marine-based ice shelf and the influence on fracture propagation: Insights from a core on the Brunt Ice Shelf 

Emma Pearce, Oliver Marsh, Liz Thomas, Alex Brisbourne, Tom Mitchell, Jack Humby, Dieter Tetzner, Manon Jones, Mishka Rawatlal, Shaun Miller, and Amy King

Fracture-induced ice shelf instability is a critical contributor to uncertainties in sea level projections, which are central to global flood mitigation planning. While the occurrence of ice fracturing at critical stress thresholds is well-documented, the mechanisms governing fracture timing, rate, and orientation remain poorly understood, particularly across ice shelves with varying ice properties and provenance. Observations on the Brunt Ice Shelf reveal unique fracture behaviours, where rifts deviate from their stress-predicted pathways to avoid blocks of meteoric ice, and preferentially fracture through thinner marine ice. The speed of propagation is also influenced by these differences in ice type.   

To improve our understanding of these fracture dynamics, a 37 m firn core through thin, marine-based ice was collected in 2024 on the Brunt Ice Shelf. This core provides a high-resolution record of precipitation and climate changes over the past 40 years, with saline layers at the base. Biogenic species within the core trace variations in summer sea ice extent and proximity to open water, including the A-81 calving in 2023, while an increasing prevalence of melt layers highlights a rise in surface melt. By integrating fracture toughness measurements from layers with varying melt and accumulation conditions, we demonstrate how climatic and environmental shifts could influence ice shelf susceptibility to fracture propagation.

How to cite: Pearce, E., Marsh, O., Thomas, L., Brisbourne, A., Mitchell, T., Humby, J., Tetzner, D., Jones, M., Rawatlal, M., Miller, S., and King, A.: Surface melt driven changes to ice properties for a marine-based ice shelf and the influence on fracture propagation: Insights from a core on the Brunt Ice Shelf, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1493, https://doi.org/10.5194/egusphere-egu25-1493, 2025.

EGU25-5893 | PICO | CR6.2

Cosmic rays detector for the measurement of snowpack by both neutrons and muons absorption 

Enrico Gazzola, Mauro Valt, Stefano Gianessi, Barbara Biasuzzi, and Luca Stevanato

The amount of water stored in mountain snowpack as Snow Water Equivalent (SWE) is notably difficult to measure due to the complexity of the snowpack and the remoteness of the areas of interest. Well-established methods include in-situ coring campaigns performed by specialized personnel, estimations by computational models usually relying on meteorological observations, and remote sensing by satellites. Each method has its own limitations, leaving a gap in temporal and spatial resolution that highlights the importance of deploying proximal sensors providing continuous SWE measurements in remote areas.

Recently, probes based on the detection of cosmic rays have emerged as a suitable candidate, with the development of devices based on either the absorption of neutrons or muons by the snowpack. The detector manufactured by Finapp is characterized by the patented feature of being able to contextually detect and discriminate both neutrons and muons with the same device.

The setup for SWE measurements is composed by a Finapp probe on the ground and a reference detector on a mast, out of the snowpack, to monitor the incoming cosmic rays flux. A network of 25 such systems has been deployed on the Italian mountains of the Veneto region, spanning elevations between 1400 and 2600 m asl, integrating them to pre-existent meteo-nivological stations managed by the Regional Environmental Protection Agency of Veneto (ARPAV).

SWE can be calculated basing on the drop of either neutron counts or muons counts by the ground detector. In this presentation we will compare the two methods, with a special attention to their notably different footprint, and the advantages of their simultaneous availability will be highlighted. The SWE trends will be also compared to field campaigns, historical trends and computational models.

How to cite: Gazzola, E., Valt, M., Gianessi, S., Biasuzzi, B., and Stevanato, L.: Cosmic rays detector for the measurement of snowpack by both neutrons and muons absorption, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5893, https://doi.org/10.5194/egusphere-egu25-5893, 2025.

EGU25-6793 | ECS | PICO | CR6.2

Testing time-lapse gravimetry on Murtèl rock glacier (Swiss Alps) to quantify subsurface water/ice storage changes 

Dominik Amschwand, Landon Halloran, Daniel Vonder Mühll, Martin Hoelzle, and Jan Beutel

Seasonal storage of liquid and frozen water in high-mountain catchments will play an increasingly important role as a hydrological buffer in rapidly deglaciating mountains, sustaining streamflow during late-summer dry phases after completion of the snowmelt. Depending on the local topo-climatic conditions, these catchments are (partly) underlain by permafrost. However, below-ground water/ice storage processes, their dynamics, and water pathways are currently poorly characterized. This holds particularly in high-mountain catchments where field data with sufficient resolution to capture the spatial variability are sparse. Among geophysical techniques, time-lapse gravimetry stands out as a method that is directly sensitive to the target quantity, mass (density) distribution changes, at an appropriate spatial scale. Time-lapse gravimetric surveys have successfully quantified groundwater storage changes in high-mountain catchments (Halloran, 2025), but have never been deployed on mountain permafrost, notably rock glaciers.
33 years after pioneering gravimetric investigation on Murtèl rock glacier (Vonder Mühll & Klingelé, 1994), we return to the site with a state-of-the-art relative spring gravimeter (Scintrex CG-6 Autograv) able to resolve water/ice storage changes at the few μGal range (corresponding to <10 cm water equivalent). First, we present results from repeat gravimetric surveys, complemented by drone-based photogrammetry, that we carried out in early and late Summer 2024. We observed significant, spatially variable gravity changes attributable to the seasonal ice loss in the coarse blocky active layer. Second, we compare our data with the 1991 measurements (Vonder Mühll & Klingélé, 1994). Finally, we discuss the strengths and limitations of time-lapse gravimetry in complex mountain permafrost terrain, including challenges related to the decomposition of the temporal gravity signal to different water and rock mass distribution changes.

References
Vonder Mühll, D. S., and Klingelé, E. E.: Gravimetrical investigation of ice-rich permafrost within the rock glacier Murtèl-Corvatsch (upper Engadin, Swiss Alps). Permafrost and Periglacial Processes, 5(1), 13–24. doi:10.1002/ppp.3430050103, 1994.
Halloran, L.J.S., Mohammadi, N., Amschwand, D., Carron, A., Gutierrez, F., Baia Sampaio, J., and Arnoux M.: Hydro-gravimetry as a monitoring solution for water and ice storage changes in dynamic alpine environments, EGU General Assembly 2025, Vienna, Austria, 27 April–2 May 2025, EGU25-3101, 2025.

How to cite: Amschwand, D., Halloran, L., Vonder Mühll, D., Hoelzle, M., and Beutel, J.: Testing time-lapse gravimetry on Murtèl rock glacier (Swiss Alps) to quantify subsurface water/ice storage changes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6793, https://doi.org/10.5194/egusphere-egu25-6793, 2025.

EGU25-6801 | PICO | CR6.2

Effect of surface cracking propagation on induced polarization of clay under freeze-thaw cycling and desiccation processes 

Haoliang Luo, Anne Jost, Julien Thiesson, Aida Mendieta, Emmanuel Léger, and Damien Jougnot

Freeze-thaw cycles and desiccation significantly influence soil surface cracking and shrinkage, reshaping pore structures and altering hydraulic properties. Despite their importance, studies using geophysical methods to evaluate how soil crack patterns and shrinkage respond to climate change remain limited. In this study, we utilized induced polarization (IP), a sensitive and non-intrusive geophysical technique, to investigate the relationship between soil surface crack patterns and complex conductivity during freeze-thaw-desiccation and desiccation-only processes. Laboratory experiments revealed that the desiccation-only sample exhibited a distinct surface texture and different types of crack intersections compared to the freeze-thaw-desiccation sample. While Y-junction-dominated crack patterns form on the sample surface during the freeze-thaw-desiccation process, the desiccation-only sample predominantly displayed more T-junctions at the crack intersections. SIP measurements revealed a sharp decline in both in-phase and quadrature conductivities below the freezing/thawing point, with high-frequency ice polarization signals emerging. During desiccation, these components exhibited an exponential decline with a consistent decay time (τ = 358 mins). Furthermore, a clear linear relationship was observed between both conductivities and surface crack ratio, as well as gravimetric water content. These findings highlight the potential of IP for monitoring crack propagation and subsurface water dynamics in clayey soils, offering a promising tool for field applications like time-lapse tomography on clayey slopes to assess water transport and structural stability.

How to cite: Luo, H., Jost, A., Thiesson, J., Mendieta, A., Léger, E., and Jougnot, D.: Effect of surface cracking propagation on induced polarization of clay under freeze-thaw cycling and desiccation processes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6801, https://doi.org/10.5194/egusphere-egu25-6801, 2025.

EGU25-8018 | ECS | PICO | CR6.2

Helicopter-borne GPR provides insights on the 2024 La Bérarde flood  

Ilaria Santin, Christophe Ogier, Raphael Moser, Huw Joseph Horgan, Antoine Blanc, and Daniel Farinotti

On 21 June 2024, the mountain settlement of La Bérarde (French Alps) was severely damaged by a flood and debris flow. Preliminary investigations conducted by the local French authorities indicate that flooding was caused by a compound event combining (i) exceptional precipitation amounts, (ii) high snowmelt rates, and (iii) a supraglacial lake outburst flood from the nearby Glacier de la Bonne Pierre. Water balance consideration, however, indicated that additional water might have come from a subsurface reservoir, possibly located within Glacier de la Bonne Pierre. To better asses this possibility, we surveyed the glacier with a dedicated Ground Penetrating Radar (GPR) campaign in November 2024. The survey used the Airborne Ice Radar of ETH Zürich (AIRETH), a dual-polarization, helicopter-borne GPR system that has been successfully applied in previous glaciological studies.

The resulting 20 km of high-quality GPR data allowed detailed imaging of the glacier’s internal structure and bedrock. We focus on the possibility for large water accumulation within the glacier, or at the ice-bedrock interface, that could have been the origin reservoir contributing to the total flood volume. Along the glacier tongue, we detected a widely distributed, high scattering zone, indicative of temperate ice containing small water inclusions. Additional evidence of a subglacial drainage network was observed, supported by both peculiar GPR features and the presence of a river outcrop at the glacier tongue, as well as possible cavities within the ice. We applied the VAW-ETHZ package WhereTheWaterFlows.jl, which determine subglacial water flow paths, to further investigate the subglacial drainage of the glacier and validate the GPR interpretation. The outcomes of this study demonstrate the value of combining advanced geophysical techniques with modelling approaches to deepen the understanding of glacier-related hazards.

How to cite: Santin, I., Ogier, C., Moser, R., Horgan, H. J., Blanc, A., and Farinotti, D.: Helicopter-borne GPR provides insights on the 2024 La Bérarde flood , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8018, https://doi.org/10.5194/egusphere-egu25-8018, 2025.

EGU25-8650 | ECS | PICO | CR6.2

Seismic monitoring of grounding line processes at Totten Glacier, East Antarctica 

Jared Magyar, Anya Reading, Ross Turner, Sue Cook, Paul Winberry, Tobias Stål, Felicity McCormack, Ian Kelly, Benjamin Galton-Fenzi, Madelaine Rosevear, Thomas Hudson, and Jason Roberts

The Aurora Subglacial Basin (ASB), East Antarctica, contains approximately 3.5m global sea-level equivalent of marine-based ice, which primarily drains through Totten Glacier. The dynamics of Totten Glacier are therefore a major influence on mass balance for the East Antarctic Ice Sheet (EAIS). The grounding line geometry is complex, and has undergone rapid migration over the past decades, with upstream regions of retrograde bed slope potentially leaving the glacier vulnerable to the marine ice sheet instability if the grounding line were to retreat beyond the Vanderford Trench. Enhanced monitoring capability for Totten Glacier, particularly in this grounding line region, is therefore of pivotal importance for assessing the future stability of the EAIS. 

Passive seismology offers a method for detecting and analysing transient or hidden glaciological processes such as stick-slip basal motion, iceberg calving, ice fracture, and subglacial hydrology. In this work, we present results from a seismic network deployed near the grounding line of Totten Glacier during the austral summer of 2018-19. Thousands of seismic events are coherently detected and catalogued across the network. We use template matching methods to compile a database of the repeating event waveforms and analyse their timing, magnitudes and inter-event durations. Such multiplet events are of particular note in this study, where the near identical waveforms are best explained by a repeating source mechanism. This is interpreted as being due to repeated slip of the glacier at asperities at the glacier bed near the grounding line. The seismic waveforms are used to investigate the underlying physics of the repeating events, comparing the underlying slipping processes active in the grounding zone to tectonic analogues. Analysis of these repeating events has the potential to elucidate the basal sliding processes key to the dynamics of this large outlet glacier. 

How to cite: Magyar, J., Reading, A., Turner, R., Cook, S., Winberry, P., Stål, T., McCormack, F., Kelly, I., Galton-Fenzi, B., Rosevear, M., Hudson, T., and Roberts, J.: Seismic monitoring of grounding line processes at Totten Glacier, East Antarctica, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8650, https://doi.org/10.5194/egusphere-egu25-8650, 2025.

EGU25-10878 | ECS | PICO | CR6.2

Radar and seismic investigations of an active glacier hydrological system in West Greenland 

Jonathan Hawkins, SIobhan Killingbeck, Matthew Peacey, Samuel Doyle, Lisa Craw, Sian Thorpe, Remy Veness, Andrew Sole, Stephen Livingstone, Neil Ross, Adam Booth, Elizabeth Bagshaw, Michael Prior-Jones, Sammie Buzzard, Laura Edwards, and Rob Storrar and the SLIDE team

A hydrologically-active subglacial lake system has been identified near the south lateral margin of Isunnguata Sermia, West Greenland. Differencing time-stamped ArcticDEM strips has revealed multiple anomalies in ice-surface elevation change. A large hydrological drainage event from Isunnguata Sermia in 2015 slowed ice flow for ~1 month and flooded the foreland, depositing up to 8 meters of sediment. Although the proglacial flooding provided evidence that the ice-surface elevation anomalies were likely caused by subglacial water bodies, satellite altimetry cannot provide direct insights into their thickness, structure and properties. Therefore, field-based geophysical measurements, including ground-based radar and active source seismics, were collected during summer 2023 and autumn 2024 to characterise the subglacial hydrological system. 

Radar data were collected in October 2024 using a 10 MHz Blue Systems Integration ice-penetrating radar (IPR) to determine ice thickness and constrain a subglacial hydrological model. 26 km of radar data were collected over two of the ice-surface elevation anomalies. The radar data cross existing airborne IPR transects and point measurements from a phase-sensitive radar (pRES). Active source seismic surveys were performed at three locations over the largest ice-surface elevation anomaly: 1) anomaly centre, 2) anomaly southern edge, and 3) between the anomaly centre and southern edge, where bright basal reflections had been identified from radar observations. Seismic data were acquired with a hammer and plate source and 48 100 Hz vertical component geophones in a 94 m-long spread at a geophone spacing of 2 m. 

Our radar results show that the ice-surface elevation anomalies overlie complex subglacial topography on the southern sidewall of the large over-deepened trough beneath the Isunnguata Sermia trunk. Across the largest surface anomaly, ice thickness varies between 380 m to 600 m. The seismic data shows a negative polarity at the ice-bed interface, coincident with a subglacial topographic low. This indicates an acoustically soft basal material, which could represent water or water-saturated sediment. Scattering and diffraction hyperbola in the radar data arise from a complex englacial structure, which have implications for attenuation of radio and sound energy. 

These observations provide new insights into the glaciology and hydrology of an important West Greenlandic outlet glacier and highlight the complexities associated with active glacier hydrological systems and their geophysical characterisation.

How to cite: Hawkins, J., Killingbeck, S., Peacey, M., Doyle, S., Craw, L., Thorpe, S., Veness, R., Sole, A., Livingstone, S., Ross, N., Booth, A., Bagshaw, E., Prior-Jones, M., Buzzard, S., Edwards, L., and Storrar, R. and the SLIDE team: Radar and seismic investigations of an active glacier hydrological system in West Greenland, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10878, https://doi.org/10.5194/egusphere-egu25-10878, 2025.

EGU25-10927 | ECS | PICO | CR6.2

Identification of spatial variations in subglacial sediment discharge and basal slip from ground penetrating radar  

Rebecca Schlegel, Lucas K. Zoet, Adam D. Booth, Andrew M. Smith, Roger A. Clark, and Alex M. Brisbourne

Basal conditions that facilitate fast ice flow are still poorly understood and their parameterization in ice flow models results in high uncertainties in ice flow and consequent sea-level rise projections. One approach to understanding basal conditions is through investigating the basal landscape of ice streams and glaciers, which has been shaped by ice flow over the underlying substrate.

In this study, we map the subglacial landscape and identify basal conditions of Rutford Ice Stream (West Antarctica) using different visualisation techniques on high-resolution 3D radar data. Our novel approach reveals bedforms of < 300 m in length, surrounded by bedforms of > 10 km in length. We assume these variations in bedform dimension to reflect spatial variation in sediment discharge. We find no correlation to glaciological factors, but our radar data reveal a correlation between variation in bedform dimension to bed composition.

We thus developed a simple model relating sediment discharge (and hence, deformation) to inferred basal condition and measurements of basal effective pressure. The model implies that effective pressure and sediment properties (low-porosity material vs soft sediment) at the ice-bed interface are first-order controls on sediment discharge and thus bedform dimensions. This work highlights the small-scale spatial variability of basal conditions and its implications for basal slip.

Assuming glaciological factors to be constant this new approach, allows spatial variation in basal conditions and effective pressure to be identified from spatial variation in bedform dimensions, observed from high-resolution radar data. This will further allow the flow mechanism to be separated into basal slip and basal deformation and a better incorporation of their variation into numerical ice flow models.

How to cite: Schlegel, R., Zoet, L. K., Booth, A. D., Smith, A. M., Clark, R. A., and Brisbourne, A. M.: Identification of spatial variations in subglacial sediment discharge and basal slip from ground penetrating radar , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10927, https://doi.org/10.5194/egusphere-egu25-10927, 2025.

EGU25-11283 | PICO | CR6.2

Characterizing rockwall permafrost dynamics at Aiguille Du Midi (French Alps) through electrical resistivity tomography monitoring  

Feras Abdulsamad, Florence Magnin, André Revil, Emmanuel Malet, Jessy Richard, Pierre-Allain Duvillard, and Ludovic Ravanel

Climate change significantly impacts high-mountains worldwide, accelerating the degradation of the cryosphere. Over the last decade, numerous rockfall events involving permafrost-affected rockwalls have been recorded, especially in the European Alps. The frequency of these events is expected to increase over time due to the degradation of mountain permafrost. This study investigates permafrost dynamics at the Aiguille du Midi (3840 m a.s.l.) in the French Alps using Electrical Resistivity Tomography (ERT) monitoring over four years. A total of three profiles each 155 m in length, were deployed downwards from the summit in three directions: north-west, south and east. A system for permanent monitoring and remote data acquisition was implemented. A time-lapse inversion technique was employed for data interpretation. Laboratory measurements of electrical resistivity were conducted on granite samples in both unfrozen and frozen conditions to evaluate the temperature-dependency of resistivity. Furthermore, temperature monitoring in three boreholes provides localized information about permafrost dynamic across the site. Our ERT results demonstrate that the temperature-dependence of resistivity in field conditions is less pronounced than in controlled laboratory settings, influenced by the complexity of the site (3D effect, human-made infrastructure, rock heterogeneity (at different scales from fractures to pores) and variable ice content. In field, the freezing temperature fluctuated between -0.5 °C and -2.5 °C. Importantly, we observed that the active layer's thickness varied significantly from one face to another, with implications for the thermal regime and potential geohazards in this mountainous environment. These results are correlated with thermal information measured in boreholes. Notably, our assessments of the hydrogeological system revealed instances of water flux, although the exact pathways of infiltration and drainage remain ambiguous. This research highlights the efficacy of ERT as a low-cost, non-invasive tool for monitoring permafrost dynamics in alpine environments and highlights the need for further methodological refinement to enhance data reliability. These findings contribute to understanding potential geohazards associated with permafrost degradation and emphasize the importance of continuous monitoring in the context of ongoing climate change.

How to cite: Abdulsamad, F., Magnin, F., Revil, A., Malet, E., Richard, J., Duvillard, P.-A., and Ravanel, L.: Characterizing rockwall permafrost dynamics at Aiguille Du Midi (French Alps) through electrical resistivity tomography monitoring , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11283, https://doi.org/10.5194/egusphere-egu25-11283, 2025.

EGU25-12160 | PICO | CR6.2

Seismic reflection surveys at GHOST Ridge, Thwaites Glacier 

Ronan Agnew, Alex Brisbourne, Sridhar Anandakrishnan, Atsuhiro Muto, Louise Borthwick, Amanda Willet, and Sierra Melton and the ITGC GHOST Team

Subglacial topography and the character of a glacier’s basal material have a controlling effect on ice flow and are therefore important to parameterise in ice sheet models. Seismic surveys provide a means to characterise basal materials through the estimation of the elastic parameters of the bed (for example, acoustic impedance and Poisson’s ratio). The subglacial topography of Thwaites glacier is oriented across flow, with a series of subglacial ridges running East to West across the glacier. The bed character in the vicinity of a subglacial ridge ~60km upstream of the grounding zone, named GHOST ridge, is of particular concern, as this ridge may be a future pinning point for the grounding zone as Thwaites retreats. We present measurements of basal conditions from an active seismic dataset acquired immediately upstream of GHOST Ridge. During the 2023-24 season a 14.4 km seismic line was shot with hot water drilled Pentolite sources. We observe varied bed topography within the 14km section, with areas of smooth bed topography interspersed with rougher areas, and crag-and-tail like features present. Bed reflectivities are consistent with a widespread subglacial dilatant till layer, with stiffer till on the stoss sides of basal topographic features, and the softest till on the lee sides of these features. We will also discuss preliminary results from amplitude-versus-offset analysis, which gives further constraint of basal elastic properties.

How to cite: Agnew, R., Brisbourne, A., Anandakrishnan, S., Muto, A., Borthwick, L., Willet, A., and Melton, S. and the ITGC GHOST Team: Seismic reflection surveys at GHOST Ridge, Thwaites Glacier, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12160, https://doi.org/10.5194/egusphere-egu25-12160, 2025.

EGU25-13020 | PICO | CR6.2

Time-lapse GPR to quantify internal glacier deformation 

Alexi Morin, Gabriela Clara Racz, Bastien Ruols, Johanna Klahold, Melissa Francey, and James Irving

The estimation of surface flow velocities using satellite imagery, photogrammetry, or GPS data is now a standard practice in glaciology. In contrast, assessing internal ice deformation remains a significant challenge, often relying upon sparse measurements and theoretical models constrained by limited data. This study explores the potential of repeat, common-offset, ground-penetrating radar (GPR) reflection surveys as a tool to address this challenge. While GPR reflection data are traditionally utilized to determine glacier bed geometry, they also reveal key information about internal glacier structures, including the distribution of air pockets, debris, and water channels. Over time, these structures deform in response to glacier dynamics, suggesting that time-lapse GPR measurements could offer insights into internal flow velocities. In this regard, we propose a localized cross-correlation (LCC) approach, inspired by feature-tracking methods, as a starting point for a non-linear inversion of the deformation field. We test our methodology on synthetic GPR profile data, where electromagnetic wave propagation is modeled in a simplified flowing glacier containing randomly distributed scatterers, as well as on repeat GPR profiles acquired on the Findelen Glacier, Switzerland. In both cases, the GPR measurements are considered along the direction of glacier flow, and the corresponding data are diffraction enhanced and migrated prior to analysis. Our findings demonstrate that the proposed approach successfully retrieves the two-dimensional along-flow velocity field, highlighting its potential for field applications and future extension to three-dimensions.

How to cite: Morin, A., Racz, G. C., Ruols, B., Klahold, J., Francey, M., and Irving, J.: Time-lapse GPR to quantify internal glacier deformation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13020, https://doi.org/10.5194/egusphere-egu25-13020, 2025.

EGU25-13161 | ECS | PICO | CR6.2

Multi-Offset Imaging of Bed Topography Using Radio Frequency over Fiber Radar Arrays: Modelling and Initial Field Results 

Daniel May, Olivers Pranis, Dustin Schroeder, Thomas Teisberg, Sameeh Maayah, Anna Morgan, Zara Rutherford, Gilberto Tovar, and Leo Hollberg

Radio-echo sounding (RES) is a widely used tool in glaciology, providing insight into englacial and subglacial environments. Conventional high-spatial resolution RES surveys typically employ zero- or small-offset configurations with a single transmitter-receiver pair. Such surveys often prioritize spatial coverage over monitoring temporal changes in englacial and subglacial conditions. Stationary radar arrays aimed at providing time series data have been previously deployed in glaciated regions to provide estimates of basal melt rates, infer vertical strain within ice sheets, and image englacial layers in 3D. However, these stationary arrays are unable to image the ice-bed interface with sufficiently high resolution to infer changes in bed geometry over time. This is largely due to hardware limitations in the radar systems used in glaciology which typically support an inadequate number of antenna elements. Unlike in towed or airborne radar systems, where spatial resolution can be improved through synthetic aperture processing techniques, the spatial resolution achieved by a stationary array is proportional to the number of real antenna elements deployed. We overcome limitations in the number of supported antennas by integrating radio-frequency over fiber (RFoF) hardware, typically used in the communications industry, into existing radar systems such as the autonomous phase-sensitive radio-echo sounder (ApRES), as well as software-defined radios (SDRs). By converting RF signals to optical signals, lossy copper-based coaxial cables is replaced by low-loss fiber optic cables, permitting large separations between receive and transmit elements without significant signal attenuation during transmission. Further, the low cost, high switching speeds, and large number of output channels provided by fiber optic switches allows for a cost-effective way to rapidly cycle through 100s of antenna elements using a single radar unit RF input or output port. These modifications allow an ApRES, which traditionally supports up to 8 receive and 8 transmit antennas, to handle 100s of antennas on both the receive and transmit side, offering significant improvements in imaging capabilities. Such a system could support advanced imaging geometries capable of 3D time-lapse monitoring of englacial and subglacial processes, such as seasonal hydrology, subglacial erosion, isostatic rebound, and the evolution of sub-ice shelf features. We demonstrate these imaging capabilities through modelling and initial field results using our modified ApRES and SDR systems.

How to cite: May, D., Pranis, O., Schroeder, D., Teisberg, T., Maayah, S., Morgan, A., Rutherford, Z., Tovar, G., and Hollberg, L.: Multi-Offset Imaging of Bed Topography Using Radio Frequency over Fiber Radar Arrays: Modelling and Initial Field Results, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13161, https://doi.org/10.5194/egusphere-egu25-13161, 2025.

EGU25-13712 | ECS | PICO | CR6.2 | Highlight

UAV-based monitoring of the mountain cryosphere: Recent advances and future prospects 

Alexander Raphael Groos

The mountain cryosphere responds very sensitively to global climate change because of local processes and positive feedbacks, with far-reaching hydrological, ecological and socio-economic consequences at different spatial scales. To uncover rapid changes, assess potential impacts and develop effective adaptation strategies, comprehensive monitoring of the state and evolution of the mountain cryosphere is essential. In recent years, unoccupied aerial vehicles (UAVs) equipped with cameras or geophysical and meteorological instruments have been increasingly deployed for detailed mapping and monitoring of the mountain cryosphere. UAVs facilitate a wide range of geoscientific applications and are particularly useful for surveying areas in alpine terrain that are difficult to access. They also have great potential for the spatial study of small-scale and dynamic processes. Using high-resolution digital elevation models or dense point clouds from (repeated) UAV surveys has become a widespread method for mapping snow depth changes and quantifying glacier volume loss. The ongoing miniaturisation of electronic sensors and the specific development of multispectral and thermal infrared cameras, GPR and LiDAR systems and other geophysical instruments for UAV-based surveys have opened up new opportunities for cryospheric research in complex terrain. Recent advances include the measurement of glacier thickness and snow depth using UAV-borne GPR, the mapping of supraglacial debris thickness and permafrost distribution using UAV-based thermal infrared thermography, the mapping of snow and ice albedo using UAV-based multispectral imaging, and the investigation of the atmospheric boundary layer over ice and snow using UAVs. Here I briefly discuss the potential and limitations of recent advances in UAV technology for cryospheric research and outline future prospects for the detailed monitoring of mountain glaciers, permafrost and snow cover.

How to cite: Groos, A. R.: UAV-based monitoring of the mountain cryosphere: Recent advances and future prospects, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13712, https://doi.org/10.5194/egusphere-egu25-13712, 2025.

EGU25-14977 | ECS | PICO | CR6.2

In-Situ Bathymetry and Volume Estimation of Glacial Lakes in Western Himalaya 

Suresh Das and Raaj Ramsankaran

In recent years, glacial lake outburst flood (GLOF) hazards in the Himalayan region have garnered considerable attention. The expansion of glacial lakes and the corresponding increase in volume play major roles in the initiation of GLOFs. Due to the lack of systematic assessments and the challenges associated with conducting field surveys, communities living downstream face significant risks from potential GLOFs. Accurate volume estimation of glacial lakes is crucial for calculating outburst flood peak discharge and simulating flood evolution. However, in-situ bathymetry-derived volume estimations are limited to only a few glacial lakes. Consequently, earlier studies have relied on volume-area empirical relations, which have shown substantial discrepancies. In this study, we surveyed four glacial lakes—Kya Tso Lake (KTL), Panchi Nala Lake (PNL), Gepang Gath Lake (GGL), and Samudri Tapu Lake (STL)—located in the Chandrabhaga basin, western Himalaya. Among these, GGL and STL are reported as potentially dangerous glacial lakes (PDGLs) due to their rapid expansion and risk of future bursts. In-situ depth measurements were conducted using an echo sounder mounted on an unmanned surface vehicle (USV) and portable inflatable kayak. The lake basin morphologies were modelled using triangulated irregular networks (TINs). We compared the bathymetry-derived lake volumes with volumes estimated using commonly used empirical equations. The results revealed maximum depths of 16 m, 10 m, 46 m, and 59 m for KTL, PNL, GGL, and STL, with corresponding storage capacities of 0.89 × 10⁶ m³, 0.44 × 10⁶ m³, 24.12 × 10⁶ m³, and 24.69 × 10⁶ m³, respectively. Substantial discrepancies (± 47-309%) were observed between volumes derived using existing empirical equations and those obtained through in-situ bathymetry for all four lakes. None of the commonly used equations produced similar volume with in-situ observations. Despite several challenges during the USV survey, like noise from variable sound penetration under different turbidity, limited telemetry, wind, boat speed relative to water depth, and floating ice on lake, this study provides valuable in-situ bathymetric data for future modelling and hazard assessment of rapidly expanding PDGLs in the region. The present study emphasizes the need for more robust, in-situ-based bathymetric datasets of glacial lakes to develop an empirical equation with better applicability.

How to cite: Das, S. and Ramsankaran, R.: In-Situ Bathymetry and Volume Estimation of Glacial Lakes in Western Himalaya, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14977, https://doi.org/10.5194/egusphere-egu25-14977, 2025.

Permafrost is warming globally as shown in many recent studies based on borehole temperature monitoring. However, data on changes in ground ice and water content in permafrost areas are scarce, which are both expected to change strongly close to the melting point when latent heat effects upon melting mask further temperature increase until all ice has melted. This is the reason why permafrost borehole temperature monitoring is in many cases complemented by geophysical surveying, such as Electrical Resistivity Tomography (ERT), due to the strong dependence of electrical resistivity on liquid water content. ERT has been successfully applied to e.g. spatially map the active layer depth, quantify ice and water content and detect and delineate massive ice bodies within the permafrost since many years. In several cases survey lines were repeated or monitored over short time-periods to identify freeze-thaw processes or identify permafrost changes over longer time periods. However, only very rarely electrical resistivity is monitored operationally by an automated station.

In recent years, automated ERT (A-ERT) systems have been specifically developed to be deployed in harsh and remote terrain, and several systems have been installed in permafrost environments within different research projects. In this study, we collect and compare first results from several of these A-ERT stations regarding data quality over a full year monitoring period, specifics of current injection and contact resistances, energy consumption and resistivity evolution over freeze and thaw cycles. The continuously monitored permafrost resistivity data are compared for several A-ERT stations in polar and mountain regions, including the Antarctic Peninsula Region, Yukon and the Northwest Territories, Svalbard, Kyrgyzstan, Greenland and the European Alps. Finally, we will present processing approaches to relate the obtained resistivity changes to changes in water content and compare them to in-situ measured temperature and soil moisture data.

How to cite: Hauck, C. and the A-ERT comparison team: Comparison of Automated ERT stations (A-ERT) for continuous monitoring electrical resistivity in polar and mountain permafrost regions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15700, https://doi.org/10.5194/egusphere-egu25-15700, 2025.

EGU25-15704 | PICO | CR6.2

CRYO-RI: snow and ice monitoring and research infrastructure for Northern Finland 

Pertti Ala-aho, Hannu Marttila, Ali Torabi Haghighi, Anne Tuomela, Riku Paavola, Toni Liedes, Veijo Sutinen, Kati Anttila, Jarkko Okkonen, and Anna Kontu

The CRYO-RI project establishes a comprehensive research infrastructure to investigate and monitor the rapid transformations in snow, ice, and frozen ground in Northern Finland. Recognizing the need to reassess historical projections and governance frameworks related to cryospheric systems, the project focuses on documenting these changes with high-quality, dynamic monitoring systems. CRYO-RI addresses this pressing challenge through a regionally focused, interdisciplinary snow and ice research infrastructure cluster. The consortium comprises the University of Oulu, the Finnish Meteorological Institute (FMI), the Finnish Environment Institute (SYKE), and the Geological Survey of Finland (GTK).

This presentation highlights the advancements in snow and ice monitoring infrastructure achieved within the CRYO-RI project. Key developments include: (i) innovative temperature-based approaches for monitoring snow, permafrost, and river ice conditions using low-cost IoT sensors, distributed temperature sensing with optical cables, and Simba equipment, (ii) updated snow field monitoring stations at the Oulanka and Sodankylä Research Stations, (iii) in-situ stable water isotope analysis of seasonal snowpacks, (iv) a river ice monitoring program, (v) GNSS-R-based snow and ice monitoring, (vi) advanced soil laboratory equipment for assessing frozen soil properties, and  (vii) UAV-based measurements using LiDAR, ground penetrating radar (GPR), and synthetic aperture radar (InSAR) sensors.

The collective efforts of the CRYO-RI consortium aim to generate novel insights, innovative measurement methodologies, and cutting-edge research at the intersection of cross-disciplinary science and cryosphere-related resource management. Additionally, the CRYO-RI platform provides open-access data and measurement infrastructure, inviting collaboration with partners from academic, public, and private sectors

How to cite: Ala-aho, P., Marttila, H., Torabi Haghighi, A., Tuomela, A., Paavola, R., Liedes, T., Sutinen, V., Anttila, K., Okkonen, J., and Kontu, A.: CRYO-RI: snow and ice monitoring and research infrastructure for Northern Finland, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15704, https://doi.org/10.5194/egusphere-egu25-15704, 2025.

EGU25-16124 | PICO | CR6.2

Towards a Unified Model for Wet Snow Permittivity 

Carlo Marin

The development of a unified model for wet snow permittivity has remained a persistent challenge in remote sensing applications. While research conducted in the 1980s and 1990s yielded permittivity models for dry and wet snow and facilitated the development of in-situ snow probes, the application of these models in practical contexts, particularly across a broad frequency spectrum, remains an area requiring further investigation. The absence of a universally accepted model for wet snow impedes accurate retrievals of essential snow properties, including density, snow height, and liquid water content (LWC), from ground-based, drone-based, and satellite radar observations. This result in inconsistencies among LWC measurements from the different systems and retrieval methods.

The primary impediment to progress in this area is the limited availability of comprehensive reference datasets encompassing simultaneous measurements of permittivity, LWC, density, and a diverse range of snow conditions. The traditional method for LWC determination, employing freezing calorimetry, offers high accuracy under controlled conditions and with skilled operators but is characterized by a time-intensive measurement process, thereby limiting the feasibility of extensive data acquisition.

This study undertakes a re-evaluation of existing field campaign data concerning wet snow permittivity at a wide range of frequencies, considering the diverse acquisition methodologies employed and their associated limitations. By critically appraising the underlying assumptions and limitations of existing permittivity models, we seek to reconcile observed discrepancies. The ultimate objective of this research is to formulate recommendations for future field campaigns, emphasizing enhanced data quality and the resolution of existing knowledge gaps that currently limit the development of robust wet snow permittivity models across a broad frequency range spanning from the MHz to tens of GHz.

Through systematic analysis and the identification of critical knowledge gaps, this investigation will contribute to the advancement of a unified understanding of wet snow permittivity, with the potential to significantly enhance the accuracy of snow property retrievals derived from remote sensing observations.

How to cite: Marin, C.: Towards a Unified Model for Wet Snow Permittivity, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16124, https://doi.org/10.5194/egusphere-egu25-16124, 2025.

EGU25-16146 | ECS | PICO | CR6.2

Cryowurst: a wireless borehole instrument for observing hydrology and ice kinematics in surging glaciers 

Lisa Craw, Michael Prior-Jones, Christine Dow, Brittany Main, Jonathan Hawkins, Hashem Alnader, Sophia M. Rahn, and Luke Copeland

Glacier surges are dramatic increases in glacial ice flow velocity occurring over short periods of time (months to years), which can lead to rapid advance of the ice front and trigger hazardous outburst flooding in local areas. Direct measurements of the basal hydrology and internal dynamics of surging glaciers are sparse, due to the limitations of wired instrumentation and the unpredictability of surge timing. Consequently, the causes of surge events are poorly understood, and we are unable to accurately predict their occurrence.

We have developed a borehole instrument, the sausage-shaped "Cryowurst", which can wirelessly transmit measurements of temperature, electrical conductivity, pressure and tilt within and beneath a glacier to the surface over a period of multiple years. These sensors allow us to directly measure the hydrological conditions and kinematics of ice deformation, over longer time periods than is currently possible with wired instrumentation due to cable breakage.

We installed a vertical string of four Cryowursts 20-50m apart in a hot-water-drilled borehole in Dän Zhùr (Donjek Glacier), a surging glacier in the Yukon territory of Canada, which is predicted to surge before 2027. We present preliminary data on the basal hydrology and internal kinematics of the glacier, which were transmitted through up to 170m of ice, and received at a solar-powered and satellite-enabled receiving station on the glacier surface. Based on recent testing, there is potential for these instruments to transmit data continuously over multiple years, capturing novel information about the causes and consequences of glacier surging.

How to cite: Craw, L., Prior-Jones, M., Dow, C., Main, B., Hawkins, J., Alnader, H., Rahn, S. M., and Copeland, L.: Cryowurst: a wireless borehole instrument for observing hydrology and ice kinematics in surging glaciers, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16146, https://doi.org/10.5194/egusphere-egu25-16146, 2025.

EGU25-16302 | ECS | PICO | CR6.2

Study of Snowpack Stratigraphy Using a SFCW Radar (0.6 – 6 GHz): Experimental Measurement and Electromagnetic Simulation. 

Adrián Subías Martín, Víctor Herráiz-López, Iñigo Salinas, Samuel T.Buisán, and Rafael Alonso

The characterization of snowpack stratigraphy is essential for understanding the physical processes associated with its evolution, assessing risks and optimizing water resource management. Non-destructive and real-time measurement systems for analyzing the snowpack structure are crucial for this characterization. This study presents reflectance measurements, as a function of the snowpack depth, using a stepped-frecuency continuous-wave (SFCW) radar. This system operates at the AEMET Formigal-Sarrios field laboratory in the Spanish Pyrenees.

The measured reflectance is compared to the simulated reflectance derived from the structure obtained through in situ experimental measurements and simulations performed using the SNOWPACK software. Simulated reflectance calculations are conducted using a matrix-based electromagnetic plane wave model.

The in situ experimental measurements of snowpack structure include the assessment of density, grain type, and hardness. At the same time, local meteorological data is used to determinate the temporal evolution of the snowpack profile through the use of SNOWPACK software. This process generated detailed profiles including density, grain characteristics, hardness and liquid water content (LWC).

The agreement between radar SFCW measured reflectance and the reflectance calculated based on the experimental measured profile and the simulated profile from SNOWPACK demonstrate that this method, which is real-time, non-destructive and doesn't interfere with the evolution of the snowpack, is able to reveal its internal structure with a high level of detail. This makes possible a clear identification of the transitions between layers with different physical properties.

How to cite: Subías Martín, A., Herráiz-López, V., Salinas, I., T.Buisán, S., and Alonso, R.: Study of Snowpack Stratigraphy Using a SFCW Radar (0.6 – 6 GHz): Experimental Measurement and Electromagnetic Simulation., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16302, https://doi.org/10.5194/egusphere-egu25-16302, 2025.

EGU25-16424 | PICO | CR6.2

Permafrost Distribution and Percolating Water at Mt. Zugspitze: Insights from Seismology including DAS 

Fabian Lindner, Krystyna Smolinski, Riccardo Scandroglio, Andreas Fichtner, and Joachim Wassermann

Degradation of mountain permafrost due to global warming reduces the stability of steep rock slopes, increasing the hazard potential for humans and infrastructure. However, detection and continuous monitoring of permafrost environments remains challenging due to the harsh conditions typically encountered in high Alpine terrain. In this study, we present results from passive seismic monitoring conducted at Mt. Zugspitze in the German/Austrian Alps.

Between 2021 and 2023, we collected continuous passive seismic data from three small seismic arrays installed along the permafrost-affected ridge to the west of the summit. This dataset is complemented by campaign-wise distributed acoustic sensing (DAS) in the tunnel systems beneath the ridge, as well as rock temperature logging and cleft water flow measurements at multiple locations near our seismic deployments.

Coda-wave interferometry reveals seasonal seismic velocity changes for most station pairs. Regarding rock temperature, pairs including stations located on the warmer south-facing slopes are primarily influenced by seasonal freezing only, whereas station pairs located on the colder north-facing slopes also indicate active-layer deepening and thus the presence of permafrost. Additionally, slant-stack analysis of DAS recordings from the northern part of the ridge also provides evidence for active-layer development during summer and fall, offering in-situ seismic observations of permafrost dynamics. Besides rock temperatures, some station pairs show a strong correlation with water flow through rock fractures, which may influence permafrost distribution.

Compared to other methods, seismology is less laborious and costly, non-invasive and allows continuous monitoring. Here, we demonstrate that it can effectively monitor freeze-thaw processes and locate permafrost. Furthermore, the results from our northern ridge deployments show evidence for extensive active-layer thaw and refreeze, indicating that permafrost may be more wide-spread than previously suggested by other studies.

How to cite: Lindner, F., Smolinski, K., Scandroglio, R., Fichtner, A., and Wassermann, J.: Permafrost Distribution and Percolating Water at Mt. Zugspitze: Insights from Seismology including DAS, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16424, https://doi.org/10.5194/egusphere-egu25-16424, 2025.

EGU25-16989 | ECS | PICO | CR6.2

Non-invasive monitoring of high-alpine snow dynamics with Cosmic-Ray neutron sensing – a case study at two locations at the Zugspitze Massif  

Paul Schattan, Nora Krebs, Benjamin Fersch, Martin Schrön, Roberta Facchinetti, Elias Bögl, Carolin Rempfer, Jakob Knieß, Karl-Friedrich Wetzel, Christian Voigt, Korbinian Achmüller, Till Rehm, Karsten Schuzl, and Franziska Koch

Monitoring snow water resources is crucial to understand the dynamics of snow-fed mountain rivers. Still, in harsh and remote environments like mountain regions using conventional measurement techniques remains particularly challenging. Cosmic-Ray Neutron Sensing (CRNS) constitutes an emerging method for autonomous and non-invasive monitoring of soil moisture and snow dynamics at intermediate spatial scales of several hectares. The method is therefore promising for monitoring snow water equivalent (SWE) in high alpine locations.

The analysis includes two sites at the Zugspitze Massif, differing in elevation and surrounding topographical features. Both sensors have been installed inside existing buildings with steep roofs to avoid snow accumulation, rather than establishing new infrastructure in complex terrain. The CRNS at the Environmental Research Station Schneefernerhaus (UFS, 2656 m a.s.l.) was installed in November 2015 in the Kugelalm located on one of the terraces. A second CRNS was installed in October 2023 in the building of “Zugspitze Geodynamic Observatory Germany” (ZUGOG) operated by the German Research Centre for Geosciences (GFZ) at the summit (2962 m a.s.l.). The CRNS signal is compared against spatially distributed reference SWE based on manual measurements, terrestrial lidar and airborne photogrammetry. Furthermore, Monte Carlo based neutron simulations using the URANOS model and a dedicated modular scenario tool (YULIA) are performed to characterize the local dynamics at the measurement sites.

First results prove that CRNS is suitable for monitoring SWE dynamics even at high alpine locations like the Zugspitze Massif. At UFS the neutron counts reveal both extremely dry years, like 2022, but also very snow-rich years, like 2019 and 2024, which were among the wettest since 2015. The high altitude, the shape of the steep topography and the rocky underground with limited soil cover reduce the statistical error and increase the seasonal dynamics in the neutron flux, facilitating CRNS based SWE monitoring. Another noteworthy aspect is, that due to the large measurement footprint of several hectares, CRNS can even be used when installed within existing buildings, thus reducing costs and limiting the environmental impact of the installation.

How to cite: Schattan, P., Krebs, N., Fersch, B., Schrön, M., Facchinetti, R., Bögl, E., Rempfer, C., Knieß, J., Wetzel, K.-F., Voigt, C., Achmüller, K., Rehm, T., Schuzl, K., and Koch, F.: Non-invasive monitoring of high-alpine snow dynamics with Cosmic-Ray neutron sensing – a case study at two locations at the Zugspitze Massif , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16989, https://doi.org/10.5194/egusphere-egu25-16989, 2025.

EGU25-19502 | ECS | PICO | CR6.2

Ice content estimation in a Palsa at Aidejavri (Norway) using High-Frequency Induced Polarization (HFIP) 

Raphael Schulz, Isabella Burger, Annika Pischke, Sebastian Westermann, and Andreas Hördt

Permafrost is an import carbon sink on earth and its thawing due to global warming is considered one of the most critical tipping points in climate change. Among permafrost landforms, palsas – frost-heaved mounds with ice-rich cores - are particularly sensitive to global warming. Palsas form under conditions of alternating freezing and thawing, leading to the accumulation of ice lenses that elevate the ground surface. As global temperatures rise, palsas are increasingly subject to degradation, which results in subsidence and the release of stored greenhouse gases, profoundly affecting local and global ecosystems.

This study focuses on a palsa located in a peat mire at Aidejavri/Norway, aiming to characterise it using geophysical methods. High-Frequency Induced Polarization (HFIP) was employed to quantify ice content across the palsa. HFIP is an innovative method that measures the frequency-dependent electrical conductivity in the frequency-range between 100 Hz and 100 kHz. In that range, the electrical permittivity of water ice exhibits a sharp decrease, making HFIP suitable for ice-content estimation. The HFIP data were inverted in 1D to isolate the polarization response of the subsurface from induction. A two-component dielectric mixture model was used to invert the data in 2D, providing detailed spatial insights into ice distribution. The results indicate high ice contents underneath the palsa, togehter with clear signs of degradation by decreasing ice contents at the edges where ponds are visible at the surface.

To supplement these findings, electrical resistivity tomography (ERT) and ground-penetrating radar (GPR) were applied. ERT revealed the lateral extent and resistivity contrasts of the permafrost, while GPR delineated the upper boundary of the frozen layer. Together, these methods provided a comprehensive view of the palsa’s internal structure.

This study shows that HFIP, paired with effective pre-processing and additional methods, serves as a dependable approach for examining ice-rich permafrost. The results can be used to characterize the current state of the palsa and provide data on ice content and spatial variability. The data constitute the beginning of repetitive measurements, that aim to capture temporal changes in the palsa’s internal structure and ice content. These repeated observations will help track the dynamics of permafrost degradation over time, offering insights into how rapidly such landforms respond to climatic variations.

How to cite: Schulz, R., Burger, I., Pischke, A., Westermann, S., and Hördt, A.: Ice content estimation in a Palsa at Aidejavri (Norway) using High-Frequency Induced Polarization (HFIP), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19502, https://doi.org/10.5194/egusphere-egu25-19502, 2025.

EGU25-19748 | PICO | CR6.2

Ice-bed interface conditions in the accumulation zone of the Grenzgletscher 

Francesca Falcini, Coen Hofstede, Olaf Eisen, and Elisa Mantelli

Ice streams are river-like features of ice sheets that move much faster than the surrounding, ice. This contrast in velocity (100s m/yr vs 10s m/yr) results from ice flow being dominated by basal sliding with a fully temperate bed within ice streams, whereas ice is sliding little or not at all outside, where the bed is below the melting point. Here, we present initial results from an ERC-funded project, PHAST, which seeks to unravel the physics driving ice stream formation and dynamics. As part of this project, we seek to characterize observationally the onset of basal sliding at cold/temperate basal transition at an easily accessible alpine glacier (Grenzgletscher). Previous research has found a cold bed in the accumulation zone and a temperate bed in the ablation zone. However, the location of the cold/temperate basal transition is not known. Using a micro vibrator Elvis 7 (p-wave generator) we collected two active seismic profiles at a 3720 m high plateau on the Grenzgletscher; one parallel (250 m) and one (325 m) perpendicular to ice flow. The parallel profile shows a surprising lack of structure below the 328m deep ice-bed contact, suggesting it is likely to be bedrock. However, at the downstream end of the profile there is some stratification, which could be eroded sediments. As there is no polarity reversal at the ice-bed contact we find no indication of water at the bed. These initial results suggest that the cold/temperate basal transition is located further downstream. However, further analysis of this data, alongside passive seismics and ground-penetrating radar data, will help us identify the transition with more confidence – assisting a drilling campaign to be undertaken in 2026.

How to cite: Falcini, F., Hofstede, C., Eisen, O., and Mantelli, E.: Ice-bed interface conditions in the accumulation zone of the Grenzgletscher, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19748, https://doi.org/10.5194/egusphere-egu25-19748, 2025.

The Magnaprobe, a widely used automated snow depth probe patented in 1999 (US Patent 5,864,059), has revolutionized the collection of snow depth data globally. By significantly increasing the speed of data collection compared to traditional methods, the Magnaprobe enables an exponential growth in data points. However, our study reveals a critical limitation: over-probing issues that can lead to substantial errors in snow depth measurements. In a comprehensive field validation study conducted in a boreal forest ecosystem in interior Alaska, we found that the Magnaprobe overestimated snow depth by up to 53.8% in certain ecotypes. These findings underscore the importance of validating Magnaprobe measurements in the field to prevent significant overestimations of snowpack depth. Our research highlights the need for careful consideration of instrument limitations and underscores the importance of ground-truthing automated measurements to ensure accurate snow depth data, which is crucial for various applications in hydrology, ecology, and climate science.

How to cite: Vas, D., Brodylo, D., and Baxter, W.: Validation of an Automated Snow Depth Probe: Addressing Over-Probing Issues in a Boreal Forest Ecosystem, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20710, https://doi.org/10.5194/egusphere-egu25-20710, 2025.

EGU25-2063 | Posters on site | ERE1.3

Salt weathering of coastal stone heritage in Mykonos, Greece 

Luigi Germinario and Claudio Mazzoli

One of the most critical challenges for preserving and protecting historical built heritage in coastal regions is the comprehension of the interaction between building materials and seawater or sea spray and its effects in time. This contribution addresses the forms and dynamics of sea salt weathering by considering as case study Mykonos Castle in Greece, built from the 13th century and now surviving only in its towers, churches, and stone walls, being just a few meters away from the shore or even underwater. The fieldwork and preliminary laboratory activities were arranged for investigating the petrographic characteristics and decay patterns of the main building stones (gneisses, marbles, granitoids, etc.), their in-pore salt content constrained by orientation, height, and distance from the sea, and rate and amount of their surface erosion monitored on site. The findings are expected to help assessing the vulnerability of cultural heritage in coastal regions due to changing environmental stresses, also in view of climate change.

 

Acknowledgements

This study is carried out within the project THETIDA, which has received funding from the European Union's Horizon Europe scheme under the program Culture, Creativity and Inclusive Society (grant agreement no. 101095253).

How to cite: Germinario, L. and Mazzoli, C.: Salt weathering of coastal stone heritage in Mykonos, Greece, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2063, https://doi.org/10.5194/egusphere-egu25-2063, 2025.

EGU25-3685 | Posters on site | ERE1.3

An assessment of GO addition to an NHL binder 

Enrico Garbin, Matteo Panizza, Maria Chiara Dalconi, Luca Nodari, Codrut Costinas, Lucian Baia, Liviu Cosmin Coteţ, and Patrizia Tomasin

Natural Hydraulic Lime (NHL) binders are generally preferred to those cement-based in case of restoration works, thanks to their good compatibility with historical substrates. Moreover, they can be considered more sustainable in comparison to cement, being sintered at lower temperatures. Nonetheless, while having a good compatibility with historic substrates, their performance might need improvement in terms of strength values and strength development without sensibly affecting their stiffness.
To this purpose, the incorporation of Graphene Oxide (GO) was considered, due to the beneficial effects showed by studies on cementitious binders. This work presents the characterization of NHL pastes (i.e. without aggregates) prepared with a water-to-binder ratio of 0.5 and 3 different dosages of GO retrieved from literature about cement and concrete, namely 0.01%, 0.06% and 0.12% by weight of NHL dry powder.
The NHL powder and the reacted binder were characterized via X-ray Powder Diffraction (XRD) and Scanning Electron Microscopy (SEM). From a mechanical standpoint, indirect tensile and compressive strengths were tested at 28 and 84 days of age, while stiffness was assessed via Ultrasonic Pulse Velocity (UPV) at 7, 14 and 28 days of age.
Preliminary results showed a minor strength improvement, which was more apparent at 84 days of age, with no remarkable modification of the stiffness. Results also indicates that it might be worth testing possible greater dosages of GO.

How to cite: Garbin, E., Panizza, M., Dalconi, M. C., Nodari, L., Costinas, C., Baia, L., Coteţ, L. C., and Tomasin, P.: An assessment of GO addition to an NHL binder, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3685, https://doi.org/10.5194/egusphere-egu25-3685, 2025.

EGU25-4351 | Posters on site | ERE1.3

A multi-analytical approach to assess potential damaged areas on the building materials of monumental structures. 

Giuseppe Casula, Silvana Fais, Maria Giovanna Bianchi, and Paola Ligas

The integrated studies within the field of non-invasive diagnostics for the characterization of the state of conservation of stone building materials of monuments have the common target to meet the current and future needs of society in the field of cultural heritage. The conservation of the built heritage requires many interventions aimed at analyzing the state of health of the monuments, their preventive preservation, reconstruction, and restoration. All actions and diagnostic analyses should respect the historical significance of the investigated monuments and the physical properties of the materials that make up the cultural heritage structures. In this context, the use of non-invasive diagnostic techniques of various nature (e.g. terrestrial laser scanner (TLS), digital photogrammetry, acoustic, electrical) plays a role of fundamental importance both in the preventive preservation and in the monitoring of monumental structures over time. In fact, the use of such techniques is also particularly effective in controlling the effectiveness of restoration interventions.

In this study we have examined different architectural elements (walls and semi-columns) of the Basilica of San Saturnino relevant monument in the historical centre of the town of Cagliari (Italy). The analysis has been carried out by different geomatic (TLS and digital photogrammetry) and geophysical (acoustics and electrical) techniques. The combined application of digital photogrammetry and terrestrial laser scanning can provide high-resolution 3D models calibrated and textured with both reflectance and natural colours useful for evaluating the state of conservation of surface materials and for rationally planning further geophysical analyses, particularly the acoustic ones carried out with tomographic methods. In this study the acoustic techniques applied in the ultrasonic range have been used essentially in two modes, namely: surface and transmission. The obtained 2D models adequately describe the longitudinal velocity distribution both on the shallow parts of the investigated old walls and on the internal section of different architectural elements (semi-columns) showing the influence of the variation of intrinsic rock properties on the ultrasonic longitudinal wave propagation. The electrical resistivity data acquired on the surface of the old walls have allowed to depict the resistivity distribution on the wall surface. Electrical resistivity is a physical property of a rock that characterizes its conductive properties. For porous media such as the building carbonate rocks under study, the electrical resistivity depends on many physical properties (i.e., internal structure, water content, fluid composition and porosity) and together with the elastic properties can be useful to interpret the various properties of the investigated materials and their conservation state. In conclusion, the non-invasive techniques applied in this study can effectively aid the restoration of the building materials at Basilica di San Saturnino, Cagliari, Italy. This study confirms how each technique gave a range of different information to the restorers, and the interventions that can be undertaken in light of the acquired knowledge of the investigated monument.

 

Acknowledgements: The authors would like to thank the Ministero della Cultura- DIREZIONE GENERALE MUSEI - DIREZIONE REGIONALE MUSEI SARDEGNA (ITALY) for their kind permission to work on the San Saturnino Basilica (Cagliari – Italy).

How to cite: Casula, G., Fais, S., Bianchi, M. G., and Ligas, P.: A multi-analytical approach to assess potential damaged areas on the building materials of monumental structures., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4351, https://doi.org/10.5194/egusphere-egu25-4351, 2025.

EGU25-8054 | Orals | ERE1.3

 The fight against shoreline erosion along the coast of the second marine station of Wimereux (France), 1899-1942 

François G. Schmitt, Virginie Gaullier, Emmanuel Blaise, and Olivier Cohen
The second marine station in Wimereux, called the Alfred Giard Zoological Station, was built at the Pointe-aux-Oies, between Wimereux and Ambleteuse (North of France), in 1899. The construction was carried out in a dune field, very close to the sea. Attached to the Sorbonne University (Paris), the station was in operation for almost 40 years, under the direction of Alfred Giard, then after his death in 1908, under the direction of Maurice Caullery. As the latter explains in his memoirs, very quickly it was necessary to build a dike to protect the building from marine erosion. Throughout the beginning of the XXth century the laboratory developed, with the construction of extensions to the building, an access ramp for a boat, and several protective dikes, including one, built by Maurice Lonquéty, who left the river mouth of the Slack at Ambleteuse 4 km North, and joined the station. In 1942 the station was destroyed by the German army.
Using archives, historical sources and old photographs, we retrace the history of this station and its fight agains marine shoreline erosion. Old airborne photographs allow the position of the station to be precisely located for the first time on modern maps, showing that it was located on what is now the foreshore, due to coastal erosion at this location. Stakes in the sand, pieces of dykes and a remains of the Lonquéty dike are still visible on the foreshore.

The lithological nature of the bedrock helps explain this differential erosion, the position of the station being on a loose area while a few hundred meters further south, the construction on the base of the Pointe-aux-Oies would have allowed the building to be protected from erosion.

How to cite: Schmitt, F. G., Gaullier, V., Blaise, E., and Cohen, O.:  The fight against shoreline erosion along the coast of the second marine station of Wimereux (France), 1899-1942, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8054, https://doi.org/10.5194/egusphere-egu25-8054, 2025.

EGU25-8233 | ECS | Orals | ERE1.3

Lead Dynamics in Black Crusts: Elemental Distribution and Mobility Analysis in Lede Stone from Antwerp, Belgium 

Sofia Deboli, Jean-Marc Baele, Alessandra Bonazza, Thibaut Van Acker, Frank Vanhaecke, Katrin Wilhelm, and Tim De Kock

Black crusts commonly form on historic buildings as a result of interactions between building materials and atmospheric pollutants. These crusts primarily consist of gypsum layers that develop on calcium-rich surfaces through sulfation processes, especially in urban environments with elevated atmospheric contaminants. Moreover, black crusts accumulate particulate matter, polyaromatic hydrocarbons, and heavy metals such as lead (Pb), largely originating from anthropogenic activities like vehicular emissions, coal combustion, and industrial operations. Acting as passive environmental samplers, these crusts offer valuable insight into urban pollution trends.

Although the water-soluble components of black crusts, such as Ca²⁺, Mg²⁺, Na⁺, and SO₄²⁻, have been extensively studied, the understanding of trace elements, particularly Pb, remains incomplete, especially regarding their behavior and mobility. This study aims to fill this gap by examining Pb distribution, availability, and interactions within black crusts and the underlying stone substrates. Samples collected from historical buildings in Antwerp were analyzed using a multi-technique approach. SEM-EDX was employed for initial chemical and morphological characterization, while LA-ICP-TOF-MS enabled the generation of high-resolution quantitative elemental distribution maps for major, minor, and trace elements. Depth-resolved analysis of Pb migration was further explored through portable LIBS, contributing to a deeper understanding of crust stratigraphy and pollutant dynamics.

Preliminary findings indicate that Pb is predominantly concentrated in the outermost layers of the black crust. Given the crust’s primary composition of gypsum, a sulfate mineral, it is hypothesized that Pb is sequestered as lead sulfates, contributing to its immobilization within the crust. However, this contrasts with existing literature, which highlights Pb’s stronger affinity for carbonate phases, suggesting a tendency for it to migrate into carbonate layers and potentially into the underlying stone substrate. The confinement of Pb within the crust deviates from expected behavior, raising important questions about its speciation. Understanding the conditions under which Pb could become mobile is crucial, with factors such as kinetic limitations, local pH variations, and environmental conditions like humidity and wet-dry cycles likely influencing its migration.

This research investigates the behavior of Pb within black crusts, aiming to advance the conservation of historic buildings while addressing the public health risks associated with urban lead exposure. By examining the factors influencing Pb mobility, the study seeks to inform the development of targeted mitigation strategies for lead contamination. The expected outcomes will not only contribute to the long-term preservation of cultural heritage but also enhance urban environmental safety, providing critical insights that bridge the fields of heritage conservation and public health.

How to cite: Deboli, S., Baele, J.-M., Bonazza, A., Van Acker, T., Vanhaecke, F., Wilhelm, K., and De Kock, T.: Lead Dynamics in Black Crusts: Elemental Distribution and Mobility Analysis in Lede Stone from Antwerp, Belgium, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8233, https://doi.org/10.5194/egusphere-egu25-8233, 2025.

EGU25-9102 | ECS | Posters on site | ERE1.3

Expert Insights on Integrating Vertical Greening Systems into Historic Buildings: Survey Findings 

Eda Kale, Marie De Groeve, Yonca Erkan, and Tim De Kock

Integrating vertical greening systems (VGS) into historic buildings presents both advantages and challenges related to heritage conservation and urban sustainability. VGS contribute environmental benefits, such as reducing surface temperatures, improving air quality, and supporting biodiversity. However, their implementation raises concerns about potential risks to architectural integrity and cultural heritage.

This study explores expert perspectives on the implementation of VGS in historic buildings, focusing on the environmental, cultural, social, economic, legal, and technical aspects. Using a mixed-methods approach, the research combines insights from a literature review with survey data gathered from experts in vertical greening and heritage conservation. Both open-ended and closed-ended responses were analyzed to identify variations in expert opinions.

The findings reveal a general recognition of the environmental benefits of VGS; however, significant technical and cultural concerns present obstacles to widespread adoption. The results emphasize the need for increased awareness and structured information for stakeholders to promote a balanced approach that maximizes the advantages of VGS while addressing the challenges associated with historic architecture.

How to cite: Kale, E., De Groeve, M., Erkan, Y., and De Kock, T.: Expert Insights on Integrating Vertical Greening Systems into Historic Buildings: Survey Findings, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9102, https://doi.org/10.5194/egusphere-egu25-9102, 2025.

Moisture has an important and essential role in the transportation of salts in masonry structures, therefore understanding the changes in moisture content provides valuable insights into the diagnostics of historic buildings, namely allowing the prediction of salt weathering. In this study, the thick walls of a fortress were studied. The Citadella is a landmark historic building in Budapest, that was built from Miocene porous limestone in the middle of the 19th century. Besides external cladding with porous limestone, the cores of the walls also contain volcanic tuffs. The walls are high (12-16 m) and their thickness is more than 1.5 m, which makes it difficult to record the moisture distribution. The sources of water are partly linked to direct precipitation on the wall surface or from capillary rise from pavement surfaces and from the soil. To assess the moisture distribution and salt content both on-site and laboratory analyses were performed during the dry summer period and wet autumn period. Not only the wall surfaces but also the subsurface zones and wall interiors were studied. Dry drillings were made to assess the in-depth moisture profile and salt content. Using an on-site moisture test it was possible to identify the moist and water-saturated zones of the ashlars and renders. Salt content and composition were measured on drilled dust samples and small samples obtained from the wall surface. Optical microscopy, XRF and XRD and Thermogravimetric analyses allowed the identification of salts. According to laboratory tests, the major salts responsible for the damage of external walls are gypsum, halite and hygroscopic nitric salts. The salt distribution within the depth shows seasonal variations. It was possible to detect the moisture distribution and salt content changes in depth and along vertical profiles. The results of the current research can be used to understand the moisture and salt distribution in thick natural stone walls and help in the diagnostics of historic structures and evaluate the salt weathering processes under various climate conditions.

How to cite: Kis, A. and Török, Á.: Seasonal changes of moisture and salt content of historic porous limestone walls; obtained form surface measurements and depth profiles, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9492, https://doi.org/10.5194/egusphere-egu25-9492, 2025.

EGU25-9880 | Orals | ERE1.3

„Alabaster from Lagny“, myth or reality? 

Wolfram Kloppmann, Undine Dömling, Lise Leroux, and Aleksandra Lipińska

Gypsum alabaster is one of the most prominent stones used in European sculpture in medieval and early modern times. Many historical quarries are documented through textual and material evidence (Lipińska, in press) but some remain enigmatic. The “albâtre de Lagny”, a town situated on the banks of the River Marne in the eastern suburbs of Paris, has been mentioned throughout the 19th century as source for sculpture, notably for the numerous altarpieces now known as English production. This is in obvious contradiction to what 20th century research found out about the workshops in and around Nottingham using local material. The systematic reference to Lagny, invalidated by material fingerprinting for those and numerous other sculptures, has discredited these earlier sources. It has even been questioned if the gypsum quarried along the Marne River has ever been used for sculpture and the Lagny alabaster was qualified as legend (Bresc-Bautier, 2018; Jugie et al., 2024).

The discovery of an unpublished manuscript, preserved at the Museum of Natural History (MNHN) in Paris, written by one of the most prominent figures of political, legal and scientific life of the late 18th century, Chrétien Guillaume de Lamoignon de Malesherbes (1721-1794) , sheds a new light on this deposit. Lamoignon provides a detailed description of an alabaster-grade layer in the gypsum quarries of Thorigny, north of Lagny, based on his personal observations and interviews with the workers, a precise stratigraphy, and a list of collected samples. He also visited a workshop in the very centre of Paris using the “Lagny alabaster”, at this time undoubtedly for decorative objects rather than for figurative sculpture. The timeframe for this manuscript is  still uncertain, we can situate it between the French translation of the “Lithogeognosia” of Pott in 1753, the 1759 alabaster essay of Daubenton, both cited by Lamoignon, and his death on the guillotine in 1794.

After transcribing the manuscript and precisely locating the historical quarry, we investigated French collections of geological reference materials and found indeed samples of “Lagny alabaster” from the 19th and early 20th century at the MNHN and the BRGM. We are currently completing our corpus of isotope fingerprints of this deposit (Kloppmann et al., 2017), so far based on a single sample provided by the Laboratory of Historical Monuments (LRMH), to better constrain its use for artwork, eventually back beyond the mid-18th century.

The Materi-A-Net project is supported by the Franco-German FRAL program (ANR-21-FRAL-0014-01 and DFG 469987104) (https://materi-a-net.uni-koeln.de/en/the-project/)

Bresc-Bautier G. (2018) La sculpture en albâtre dans la France du XVIe siècle. Revue de l’Art, 200/2018-2, 37-45.

Jugie S., Leroux L., et al. (2024) L’albâtre et ses sources : incertitudes historiques et ambiguïtés de la documentation levées grâce aux analyses. Technè, 57, 49-59.

Kloppmann W., Leroux L., et al. (2017) Competing English, Spanish, and French alabaster trade in Europe over five centuries as evidenced by isotope fingerprinting. Proceedings of the National Academy of Sciences, 114, 11856–11860.

Lipińska A. (in press) Alabaster. Studies in Material Meaning(s), Studies in Art and Materiality, Leyde, Boston: Brill.

How to cite: Kloppmann, W., Dömling, U., Leroux, L., and Lipińska, A.: „Alabaster from Lagny“, myth or reality?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9880, https://doi.org/10.5194/egusphere-egu25-9880, 2025.

One of the most visited historical sites of Budapest is the Heroes’ Square, where a 36 m high Corinthian-style stone column forms part of the Millennium Monument. On the top of the column, a bronze statue depicting Archangel Gabriel is visible. The monument was inaugurated in 1901. The stone column consists of ring-shaped limestone segments (drums). In the conical shape, the drums have a diameter of 2.25  at the lower part of the column, which reduces to 1.9 m at the top. Each drum is 0.5 m high. The condition of the stone column has aggravated in the past 120 years and the current research provides an overview of the actual condition of the stone elements and gives some hints on the preservation of the bronze statue. Tests included the on-site identification of major lithotypes, and testing surface strength and weathering grade using a Schmidt hammer. The moisture distribution was detected using a portable moisture meter. Small samples were collected for laboratory analyses and oriented samples were taken representing the north, east, south and west directions, with different exposure to sun and precipitation, representing different micro-climates. Textural analyses of samples were made by using optical microscopy and SEM-BSE, while mineralogical composition and elemental analyses were performed using XRF and thermogravimetric analyses. The prevailing lithotype is Pleistocene travertine with some textural varieties. The most common weathering forms are black crusts, dissolution features, and green staining of the stone surface from dissolved bronze. The composition of weathering crusts differs from the orientation, namely wind and rain-exposed parts have a different composition than the sheltered ones. The stability of the column was also analyzed. During structural analyses, a minor amount of cracks were also recognized. Loss of renders and dissolution of the stone surface can also cause problems. The study provides an example of integrated research of material properties and structural stability of historic stone structures.

How to cite: Török, Á. and Kis, A.: Diagnostics and preparation of restoration works of a 36 m high stone column holding a giant bronze statue, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10376, https://doi.org/10.5194/egusphere-egu25-10376, 2025.

The present study investigated the relationship between the Salt Weathering Index (SSI) (Yu & Oguchi, 2010) and WAC, which is one of the methods used to evaluate the physical properties of stone, using various salt weathering experiments on building stones and artificial stones. The stone types studied were tuff (Oya stone, Towada stone, Ashino stone, Nikka stone, Tatsuyama stone), granite (Makabe stone), sandstone (Tago stone, Indian sandstone), porous rhyolite (Koga stone), and brick. Of these, 10 types of bricks, both homemade and commercial, were used. As a result, there was a rough correlation between SSI and WAC, and the multiple linear approximation had the highest coefficient of determination. The reason for the variation in the approximation formula is the difference in rock structure. In other words, for porous rhyolite and some bricks, which were probably fired at high temperatures, the WAC value was higher than the SSI value, whereas, for sandstone and dense tuff which were formed at low temperatures, the WAC value tended to be lower. In addition, the highest coefficient of determination between the rate of dry weight loss (DWL) and the SSI was obtained in the salt weathering experiment using a total immersion method with Na2SO4, MgSO4, and Na2CO3 solutions. This is probably because the MgSO4 solution has the highest viscosity and crystallization occurs in the deeper layers, which flake off on re-immersion. For Na2SO4, the coefficient of determination is high, except for the Tago sandstone. Although the reason for this is unclear, it is considered that the Na2SO4 precipitated dissolved before it had time to grow sufficiently. In the case of Na2CO3, the DWL is high in the Indian sandstone, but this is thought to be because the quartz that makes up the sandstone dissolved in the alkaline solution.

How to cite: Oguchi, C.: Salt Susceptibility Index for various building stones and their practical durability, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12344, https://doi.org/10.5194/egusphere-egu25-12344, 2025.

EGU25-12731 | Posters on site | ERE1.3

Improving the sustainability of lime mortars by reusing cow hair 

Eduardo Molina-Piernas, María Jesús Pacheco-Orellana, Javier Martínez-López, Salvador Domínguez-Bella, and Ángel Sánchez-Bellón

In many countries, construction, agriculture and livestock sectors produce and emit a large amount of waste and greenhouse gases, accelerating the climate change. For that, new trends and policies for waste management are required due to the high and constant demand for natural resources. The recent activities framed in the green economy are favouring the reuse and recycling of many waste products, in the so-called “Zero Waste” initiatives to reduce the carbon footprint, as well as to the reduction of associated energy expenditure. Among these waste products, those linked to animal by-products not intended for human consumption are usually incinerated for their elimination in Spain, contributing to the emission of CO2. Consequently, new initiatives are required to promote the reuse of this waste, such as in the development of more sustainable construction products. This paper presents the new results of the SoSCal Project, comparing sets of lime mortar with a proportion of cow hair of 0%, 0.5%, 1%, 2%, 5%, 10% and 12% in weight per kilo of mortar. Some of the advances achieved are that, regardless of the amount of hair added, no cracking process has been observed and the amount of water required can be reduced by 5%, so that extrapolation to larger production quantities would result in significant savings. Although it is necessary to carry out more tests since the workability is compromised, and therefore it will be important to find conditions according to the need for the applicability of the mortar. Another aspect is the increase in the resistance to crystallization of salts with respect to the mortar without fibres, although the durability has been greater in practically all cases, regardless of the quantity of fibres. The addition of hair has affected the thermal properties, specifically the heat transmissivity through the samples, showing a direct relationship between the percentage of added hair and this parameter. The maximum recorded temperatures differed by almost 8°C between the samples without fibres (0%) and those containing 12% of hair after one hour of heating, with the latter also cooling down much faster due to the higher hair content. Based on the results obtained, the addition of animal fibres is showing very positive results compared to the reference mortar. Thus, enhancing the properties of a traditional product, such as lime, compared to Portland cement will also have a very positive effect, since it could reduce the production of this type of cement by having other options, which would also imply reducing the emission of CO2 into the atmosphere. However, it is necessary to continue with the tests already started and to carry out other tests, especially mechanical and weathering durability tests to evaluate its performance.

 

Acknowledgements: This study was financially supported by the Research Project TED2021-132417A-I00 funded by MCIN/AEI /10.13039/501100011033 and by the European Union NextGenerationEU/ PRTR

How to cite: Molina-Piernas, E., Pacheco-Orellana, M. J., Martínez-López, J., Domínguez-Bella, S., and Sánchez-Bellón, Á.: Improving the sustainability of lime mortars by reusing cow hair, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12731, https://doi.org/10.5194/egusphere-egu25-12731, 2025.

EGU25-13034 | ECS | Orals | ERE1.3

Exploring Daylight Optimization Policies in the Conservation and Restoration of Historical Buildings in Belgium 

Nurefşan Sönmez, Arzu Cılasun Kunduracı, and Yonca Erkan

Daylight is crucial for providing visual comfort, supporting well-being, and creating an energy-efficient environment. However, its integration into historical building conservation remains a vital yet underexplored area, requiring a delicate balance between improving occupant comfort and preserving the historical significance of these buildings.
This research investigates how daylight use is addressed in conservation policies and regulations within Belgium, with a focus on the Flanders region. The study employs a mixed-method approach, combining interviews with professionals in architecture, conservation, and built heritage with a comprehensive review of existing national, regional, and local regulations. These methods aim to evaluate the adequacy of current policies and explore opportunities for improvement.
Key questions addressed include: Which regulations and guidelines govern daylight considerations in restoration efforts? What are the most frequently altered building elements during restoration, and how does daylight integration factor into these changes? Additionally, the study probes the balance between preserving historical authenticity and adapting buildings for contemporary use, assessing whether local policies adequately support this equilibrium.
Findings reveal that while daylight optimization is increasingly recognized as essential for improving occupant comfort, energy efficiency, and the functionality of re-functioned historical buildings, its integration into conservation policies requires greater emphasis. The research highlights the need for interdisciplinary collaboration, such as architects and heritage conservationists working with environmental scientists to design innovative daylighting systems, alongside the development of more comprehensive daylight guidelines aligned with the unique requirements of historical buildings.
By exploring potential improvements to existing policies, this study aims to contribute to a more holistic approach to the restoration of historical buildings, ensuring that they remain both culturally significant and sustainably functional in modern contexts.

How to cite: Sönmez, N., Cılasun Kunduracı, A., and Erkan, Y.: Exploring Daylight Optimization Policies in the Conservation and Restoration of Historical Buildings in Belgium, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13034, https://doi.org/10.5194/egusphere-egu25-13034, 2025.

Marine geology is a relatively young discipline compared to the research conducted on land. In France, while the first draft of a geological map dates back to the 18th century (Guettard, 1746), it wasn't until 1980 that marine data on the metropolitan continental margins were integrated into the geological map at a 1/1,500,000 scale, published by the BRGM. Jean-Étienne Guettard, a physician, botanist, and mineralogist, and a friend of Lavoisier, already had the remarkable intuition of a continuity in geological formations across the English Channel. In 1917, Stanilas Meunier, in his "Geological History of the Sea," boldly claimed that the science of marine geology had French origins.

For a long time, the progress of marine geology was constrained by the barrier of the water column. Therefore, initial information about fossil seas came from land-based studies. In Northern France, particularly along the Boulonnais coast, pioneering work was carried out by Pierre Pruvost (1921, 1924) and Auguste-Pierre Dutertre, the latter writing in 1925 a geological report on Pointe aux Oies and the vicinity of the Wimereux Zoological Station in the Glanures Biologiques, published on the occasion of the Station’s fiftieth anniversary (1874-1924).

Louis Dangeard, one of the great pioneers of French marine geology, was the first in the world to publish a thesis in 1928 on a submarine basin, specifically that of the English Channel, after spending 7 consecutive years (1922-1928) aboard the prestigious research vessel “Pourquoi pas ?” under Captain Jean Charcot. Subsequently, in 1933, he succeeded in forming a team of researchers and students to establish the Marine Geology Center of Caen. In France, the first sheets of the sedimentological underwater map of the Atlantic continental shelf of France at a 1/100,000 scale were published in 1968 by the National Geographic Institute, with a remarkable contribution from Louis Dangeard’s former students: Jacques Bourcart and André Guilcher, along with Gilbert Boillot, Pierre Hommeril, Félix Hinschberger, Pierre Giresse, and Claude Larsonneur, working on state thesis topics focusing on the English Channel.

Subsequent work would be closely tied to technological advancements in marine tools, particularly geophysics, after the first oceanographic expeditions of the N/O Challenger (1872-1877). Using archives and historical sources, we trace here the evolution of marine geological cartography, a brief history of oceanographic vessels, and the exploration tools that gradually shaped the tectono-sedimentary understanding of the English Channel.

How to cite: Gaullier, V.: Birth and Evolution of Marine Geological Cartography: Contribution to the Tectono-Sedimentary Understanding of the English Channel, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15133, https://doi.org/10.5194/egusphere-egu25-15133, 2025.

EGU25-15240 | ECS | Orals | ERE1.3

Implications of green façades on historic building materials 

Marie De Groeve, Eda Kale, Scott Allan Orr, and Tim De Kock

Cities are increasingly implementing nature-based solutions (NbS) to mitigate current climate stressors in urban environments, e.g. elevated temperatures and air pollutions levels. Among NbS, ground-based green façades are well-known for their ability to cover a large surface area of vegetation while using minimal ground space. This green initiative consists of climbing plants growing along a vertical surface by either attaching themselves to the surface or using a climbing aid.

Despite the proven benefits of green façades, historic buildings, crucial components of urban environments, are often neglected in urban mitigation strategies. Concerns about potential adverse effects of greening on materials durability and structural integrity, which is currently poorly understood, have limited their implementation on historic buildings. Our research aims to understand the impact of green façades on the degradation processes of historic building materials to unlock the co-benefits of greening built heritage and to explore the potential of green façades as a preventive conservation method.

To achieve this, we analyse the interaction of green initiatives and stone-built heritage in both outdoor and controlled environments. Case studies conducted in the historic city centre of Antwerp (Belgium) over the past two years provided valuable insights on how green façades have an impact on the local microclimate. Monitoring a wide range of environmental parameters, relevant for common degradation processes of built heritage, e.g. surface and air temperature, solar irradiation,  moisture content, amount of wind-driven rain and relative humidity, enables an understanding of the mechanisms of green façades responsible for changes in the local microclimate and identifies the key extrinsic and intrinsic factors affecting the effectiveness of this greenery.  

Our findings highlight the potential of green façades to reduce the risk of common degradation processes affecting built heritage. Green façades significantly reduces solar irradiation and moisture accumulation on wall surfaces, thereby lowering the risk of biodeterioration. It also lowers the maximum surface temperatures by providing shade and tempers the relative humidity fluctuations. This buffering effect reduces the likelihood of salt crystallisation, most common during summer. In winter, evergreen vegetation enhances resistance to freeze-thaw cycles by maintaining higher minimum surface temperatures through thermal blanketing and reducing moisture accumulation on wall surfaces.

This research provides valuable insights into the potential of green façades as a sustainable and preventive conservation method for stone-built heritage. By buffering environmental conditions at the wall surface, green façades can unlock co-benefits: improving urban environments while enhancing the durability of historic building materials. A deeper understanding of the behaviour of green façades on the degradation of historic building materials can support their implementation in urban environments, ensuring that stone-built heritage becomes more resilient to current and future climate challenges.  

How to cite: De Groeve, M., Kale, E., Orr, S. A., and De Kock, T.: Implications of green façades on historic building materials, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15240, https://doi.org/10.5194/egusphere-egu25-15240, 2025.

EGU25-16284 | Posters on site | ERE1.3

Comparative analysis of digital markers in photogrammetry and laser scanning for documentation of archeological immovable monuments 

Lyubka Pashova, Ivan Lirkov, Miglena Raykovska, Nikolay Petkov, Pavel Georgiev, Kristen Jones, Hristina Kabadzhova, Georgi Evtimov, Georgi Vasilev, Stanislav Harizanov, and Milen Borisov

Advances in the accessibility of surveying and geoscience tools and developments in computer science have led to significant growth and rapid developments in the efficiency and accuracy of heritage documentation practices from objects to entire buildings and complexes. Modern cultural heritage research relies heavily on producing accurate 3D models using digital documentation methods such as photogrammetry and laser scanning. Innovative approaches to 3D documentation through digital photogrammetry and laser scanning provide the opportunity to create digital twins of real cultural heritage monuments. For these digital twins to be relatable to the real world for quantitative analysis, they must be scaled and oriented in some way. The most common method for accurately scaling 3D models is through the use of markers. Markers ensure accurate spatial measurements by linking coordinates in the model to real-world coordinates. These markers help in image orientation, calibration, and 3D reconstruction. Despite their common use, currently, there is no set of designed markers that can be universally used across various modeling methods and software. The present investigation aims to identify different types of markers used for commercial and research purposes, comparing and contrasting their type, accuracy, and suitability for specific applications. Based on an evaluation of existing software solutions and indicators through laboratory tests, the qualities of markers will be analyzed and evaluated to facilitate precise 3D modeling and improve the reliability of data collected through photogrammetry and laser scanning. The effectiveness of markers will be analyzed through comparative studies investigating how different configurations and types of markers affect the overall accuracy and effectiveness of reconstructed 3D models of photographed objects. The findings are intended to provide insight into best practices for selecting and implementing markers in archaeological surveys, contributing to more accurate and reliable results from modeling, creating newly developed innovative markers, and allowing broader applicability for precise 3D modeling of photographed national cultural heritage sites.

Acknowledgments: The authors would like to thank the Bulgarian National Science Fund for funding the research under the project  "An integral approach in creating digital twins of archeological immovable monuments using innovative technologies", contract КP-06-Н82/1 - 06.12.2024.

How to cite: Pashova, L., Lirkov, I., Raykovska, M., Petkov, N., Georgiev, P., Jones, K., Kabadzhova, H., Evtimov, G., Vasilev, G., Harizanov, S., and Borisov, M.: Comparative analysis of digital markers in photogrammetry and laser scanning for documentation of archeological immovable monuments, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16284, https://doi.org/10.5194/egusphere-egu25-16284, 2025.

EGU25-17798 | Posters on site | ERE1.3

Preliminary proposal for an experimental method to measure erosion susceptibility of heritage stones 

Javier Martínez-Martínez, Edgar Berrezueta, David Benavente, and Timea Kóvacs

Rock erodibility is an intrinsic property defined as the vulnerability of a rock to erosion (Martínez-Martínez et al., 2024; doi: 10.1201/9781003429234-177). Intuitively, erodibility is a key concept in cultural heritage conservation, especially in studies concerning the exposure of building materials to wind, rain, hail, and human activity. However, research on its implications for heritage conservation remains scarce.

Abrasion resistance of rocks is a property routinely measured in geomechanical laboratories and it offers a practical approach to assessing the erosion susceptibility of the material. Two standardized methods, the Böhme abrasion test and the Wide Wheel Abrasion test, are widely used to evaluate abrasion resistance in dimension stones. However, these methods require both large and numerous samples, rendering them unsuitable for cultural heritage studies, where sampling is severely limited. To overcome this limitation, a modified version of the Böhme abrasion test is proposed. This adaption uses a plate grinding machine commonly employed for preparing rock thin sections, making the procedure widely accessible in geoscience laboratories.

The standardized Böhme Abrasion test requires cubic samples of 71 mm size, place on a grinding plate and subjected to an abrasive load of 294N for 16 cycles of 22 turns each. Wear is calculated from the loss in volume and weight. In contrast, the modified procedure uses smaller prismatic samples (20×30×30 mm) and a plate grinding machine operating at 30 cycles per minute under a load of 0.02 N/mm². Sample dimensions and weight are measured at the beginning of the test. Each sample is abraded for 15 minutes on two perpendicular surfaces, and the final dried weight is recorded (Martínez-Martínez et al., 2017; doi: 10.1016/j.buildenv.2017.05.034). Material loss is quantified as the modified Böhme Abrasion Loss (mBAL), calculated using the equation

mBAL = ΔV = Δm/ρb

where ΔV is the volume loss (in mm3); Δm is the mass difference (in g); and ρb is the bulk density of the rock.

This modified procedure was validated using a variety of commercial dimension stones, including limestones, marbles, travertines, tuffs, calcarenites, calcirrudites, sandstones, quartzites and slates. Results where compared to those obtained with the standardized Wide Wheel Abrasion test on the same rock types. A strong correlation (R2=0.87) was observed between the two methods, expressed by the equation

mBAL = 8.9 Tww – 86.5

where Tww the wear trace measured in the Wide Wheel Abrasion Test.

This modified approach offers a viable solution for assessing erosion susceptibility in heritage contexts, enabling reliable quantification with minimal material requirements. It offers a valuable tool for developing effective conservation strategies for cultural heritage.

This work was supported by grant numbers PID2020-116896RB-C21 and PID2020-116896RB-C22 funded by MCIN/AEI/ 10.13039/501100011033

How to cite: Martínez-Martínez, J., Berrezueta, E., Benavente, D., and Kóvacs, T.: Preliminary proposal for an experimental method to measure erosion susceptibility of heritage stones, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17798, https://doi.org/10.5194/egusphere-egu25-17798, 2025.

EGU25-18457 | ECS | Orals | ERE1.3

Climate-induced Risk Assessment of Library Collections within Dora I WWII Bunker in Trondheim, Norway 

Giulia Boccacci, Francesca Frasca, Chiara Bertolin, Tonje Dahlin Saeter, Erlend Lund, and Anna Maria Siani

Short- and long-term variability in indoor microclimate conditions within conservation spaces (museums, galleries, archives, and libraries) can exacerbate the risk of deterioration of cultural materials. Active microclimate control systems are often installed to stabilize thermo-hygrometric conditions, conversely, massive buildings with thick walls are less affected by outdoor conditions due to their high thermal inertia. Historic reinforced concrete structures, like bunkers and fortifications, are often windowless, further providing stable microclimate and protecting sensitive materials from photodegradation. World War II (WWII) bunkers often labeled as “dark” or “painful heritage”, were initially perceived only as symbols of war and occupation, leading to neglect and material deterioration over time. However, the impossibility of their demolition gradually encouraged interest towards their reuse, raising awareness of their social, historical, and economic potential. This contribution provides a comprehensive microclimate analysis to support management strategies in a unique case study: the NTNU (Norwegian University of Science and Technology) library for cellulose-based materials, hosted within “Dora I” WWII bunker in Trondheim, Norway (63.43° N 10.40° E). The archive spans 3700 m2 and contains around 5200 m3 of collections, including ancient volumes, journals, newspapers, and pictures. “Dora I”, a massive reinforced concrete German submarine and terrestrial fortification with 3.5 m-thick walls, covers a total area of approximately 16,000 m². 10 thermo-hygrometers compliant with European standards were installed, ensuring representativeness of indoor conditions across two floors. Time series of air temperature (T) and relative humidity (RH) are significantly longer (7 years, since 2018) than most studies in the literature, and are continuous and complete with minimal number of missing values. Statistical approaches from climatology are applied to analyse T-RH data, decomposing time series into short-term (daily/noise) and long-term (seasonal) variability (extracted by sinusoidal fits) to provide insights into indoor climate dynamics. A comprehensive conservation risk assessment, based on dose-response functions, evaluated biological and chemical threats to archival materials using both raw and filtered (i.e., “clean”) microclimate data. This approach allows to examine how anthropogenic factors (e.g., access and archival management) in the noisy signal may exacerbate climate-induced conservation risks. The findings demonstrate the exceptional features of this massive building, where peak summer temperatures occur indoors 2 to 2.5 months later than outdoors, depending on sensor location. The study estimates no biological risks for cellulose materials from humidity-dependent insects or mould growth, with temperature-dependent insect degradation that remains a threat, particularly from June to December (although it has decreased over time). Chemical degradation risks, confirmed by three indicators, remains significant from July to October. This is evident when considering raw microclimate data, which reveals slight but still significant variations in risky days compared to "clean" data, suggesting a potential influence of human activities related to archival management. In conclusion, the findings underscore the benefits of massive structures in preserving vulnerable materials and a useful methodological approach in combining raw and filtered microclimate data to assess conservation risks. Analysing noise signal may inform conservators about the impact of their management practices, offering a useful framework for similar archival contexts worldwide.

How to cite: Boccacci, G., Frasca, F., Bertolin, C., Dahlin Saeter, T., Lund, E., and Siani, A. M.: Climate-induced Risk Assessment of Library Collections within Dora I WWII Bunker in Trondheim, Norway, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18457, https://doi.org/10.5194/egusphere-egu25-18457, 2025.

EGU25-18921 | ECS | Orals | ERE1.3

Understanding some of the effects of shelter design on deterioration at the Mnajdra Megalithic Temples of Malta 

Rosangela Faieta, JoAnn Cassar, Mantas Valantinavičius, and Daniel Micallef

The site of Mnajdra, one of the UNESCO-listed Megalithic Temples of Malta (https://whc.unesco.org/en/list/132)  dating back to 3600 - 2400 BC, is located on the southern coast of the Maltese archipelago. This site, along with two other similar sites, was sheltered in 2009 with reversible, open-sided shelters, with the aim of mitigating the critical impact of the aggressive marine environment on the conservation of the limestone megaliths.  Environmental conditions such as rain, wind, salt damage and direct insolation - triggering thermoclastism (thermal stress)- were identified as a key factor contributing to the progressive stone weathering and are currently being monitored by a multidisciplinary study.

This abstract will focus on understanding the impact of these protective, open-sided shelters on the temperature variations of the Mnajdra’s façade, with particular attention to diurnal and seasonal fluctuations, comparing to data available from the pre-sheltering period. Other studied environmental factors will not be addressed here.

The Mnajdra complex is widely recognized for its astronomical alignment, with the main (eastern) façade oriented to mark the equinoxes, solstices, and other solar events. In order to retain the association of the Temples with these alignments and to continue to observe these events, the shelters were designed to remain more open on the eastern side. As a result, surface temperature variations are currently monitored on the eastern façade, where direct sunlight could cause significant temperature fluctuations with possible subsequent deterioration effects such as microcracks formation and progressive material weakening.

Thermal imaging data was thus collected across two seasons - autumn (9th October 2023) and summer (19th June 2024) at 10-minute intervals during morning hours to identify trends of the fluctuations.

Results from these two campaigns revealed significant surface temperature fluctuations in autumn and lower variations in summer. Surface temperature gradients were observed, with a more intense gradient in autumn (from 27,8°C at 7.50 am to over 35°C at 8.50am), and less intense fluctuation in summer (from 27,3°C at 6.50am to 30,4°C at 7.50am). In both seasons, hotspots were identified particularly in areas of different megaliths (of the same stone type) where prolonged exposure (approximately 1h) to direct solar radiation occurred.

Taking into account the difference in air temperature recorded during the acquisition (19-25°C in October and 26-32°C in June) this difference can possibly be attributed to the inclination of the sun. The more significant surface temperature fluctuations observed in autumn are likely attributed to the angle of solar incidence at that time. The sun reaches the studied megaliths more directly in autumn and less directly in the summer solstice, resulting in greater variations in surface temperature.

This study forms part of a broader multidisciplinary project integrating non-invasive analytical techniques and environmental parameter modelling to evaluate the efficacy of sheltering systems. All the findings will provide scientific data to inform conservation strategies also aiming at mitigating the progressive weathering on these unique heritage sites, and ensuring their long-term preservation sites also in projection of increasing challenges due to the impacts of climate change.

How to cite: Faieta, R., Cassar, J., Valantinavičius, M., and Micallef, D.: Understanding some of the effects of shelter design on deterioration at the Mnajdra Megalithic Temples of Malta, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18921, https://doi.org/10.5194/egusphere-egu25-18921, 2025.

EGU25-19597 | Orals | ERE1.3

Assessment of UNESCO Cultural Heritage Sites Vulnerability through Multicriteria Analysis 

Diana Popovici, Andreea Andra-Toparceanu, Florina Chitea, Iuliana Armaș, Adriana Bianca Ovreiu, Sonia Malvica, and Donatella Carboni

Recognizing the inestimable value of the UNESCO World Cultural Heritage Sites for future generations, it is necessary to be aware of their vulnerability to multi-risks in the context of global climate change and the growing interest and engagement of citizens and stakeholders.

Romania is home to nine categories of cultural heritage sites (CHSs) – the Horezu Monastery, the Churches of Moldavia, the Villages with Fortified Churches in Transylvania, the Dacian Fortresses of the Orăștie Mountains, the Wooden Churches of Maramureş, the Historic Centre of Sighişoara, the Roșia Montană Mining Landscape, the Brâncuși Monumental Ensemble of Târgu Jiu, and the Frontiers of the Roman Empire – Dacia.

This work has been partially developed in the frame of two projects: 10101/2024-UB SPAH, funded by the University of Bucharest, which emphasizes sustainable and participatory activities in heritage-aware communities facing geographical risks, and 395080/2024 GeoAlliance, titled “Driving Sustainable Urban Futures:  A Romanian-Norwegian Innovation Geophysical Alliance for Green Transition and SMART City Development”. Supported by the EEA and Norway Grants, the latest project provided geophysical data for representative sampling urban of cultural heritage sites, underscoring the significant role that geophysics play in enhancing urban resilience. Results were integrated within a multi-criteria analysis (MCA) to assess the vulnerability of CHSs in Romania to both natural and man-made hazards. To apply the multicriteria analysis of CHSs vulnerability, a GIS database was developed with both natural and human-induced processes such as earthquakes, landslides, floods, that threaten the cultural heritage proprieties, being identified, mapped and ranked. This was followed by mapping the multi-hazard susceptibility features across the nine categories of the UNESCO World CHSs. The next step involved inventorying the specific attributes of each cultural heritage site that contribute to their vulnerability to various hazards and impact their resilience.  The vulnerability assessment considered several intrinsic factors that can increase exposure to hazards. Key factors include the age and the height of the structure, the elevation and the level of insulation, the used construction materials, and foundation depth. Additionally, the effectiveness of modern infrastructure, especially the underground water pipes and sewage performance, along with shallow hydrogeological and geophysical induced changes, significantly influences their risk. Other important considerations included visitor numbers and the degree of degradation of the construction, as well as ongoing consolidation and renovation efforts.

The findings from multicriteria analysis revealed the most susceptible cultural heritage sites to both natural and human-induced hazards. The paper emphasizes that although many heritage sites are highly exposed to multiple hazards, some of these sites have lower vulnerability despite being susceptible to these threats. Additionally, certain hazard processes that initially seem harmless to the CHSs are long-term damage. The results of the present work can serve as a valuable resource for site managers, enabling them to better understand where the vulnerabilities of their managed site reside and to intervene with higher efficiency in day-to-day monitoring and maintenance. Additionally, the insights can assist central and local authorities in comprehending financial requirements and allocating the necessary budget for protection and management efforts in order to strengthen CHSs protection.

How to cite: Popovici, D., Andra-Toparceanu, A., Chitea, F., Armaș, I., Ovreiu, A. B., Malvica, S., and Carboni, D.: Assessment of UNESCO Cultural Heritage Sites Vulnerability through Multicriteria Analysis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19597, https://doi.org/10.5194/egusphere-egu25-19597, 2025.

EGU25-20444 | Posters on site | ERE1.3

Archaeometrical characterization of the Roman wall paintings from Gades (Cádiz, Spain). 

Salvador Domínguez-Bella, Macarena Lara Medina, Maria Angeles Pascual Sanchez, and Eduardo Molina-Piernas

In Roman Baetica and specifically in the city of Gades (Cádiz, Spain), studies about Roman mural paintings has been mainly approached from a traditional perspective, with specific exceptions where archaeometric studies have been carried out on this type of construction and decorative materials. During an archaeological intervention carried out in the Santa Bárbara car park in Cádiz between 2009 and 2012, several Roman mural paintings fragments from the levels of waste deposits were documented. The archaeological record has allowed the levels to be dated between the 1st century BC and the 1st century AD., thus this set of pictorial remains belongs to the Republican phase or to the initial stage of the Augustean period of Gades, a period with hardly any examples of pictorial representations from the early times in Baetica. Due to the number of fragments of Roman paintings with a great variety of colours, several analytical methodologies to know the composition, technique and quality of the paintings were carried out by means X-ray diffraction, X-ray fluorescence spectroscopy, Raman spectroscopy, FTIR, polarized optical microscope, scanning electron microscope, cathodoluminescence microscope and spectrophotometry. A representative set of 31 samples was chosen for this study. Some samples only show a single layer of paint on the mortar, but it is more frequent to find several overlapping layers. The colour palette presents: light and dark blue; bright, light and dark red; purple; light and dark yellow; light green and green; white, brown and lampblack. These colours were identify as egyptian blue, cinnabar, hematite, iron ochers, celadonite, calcite, black, and mixtures between them. On the other hand, the mortars characterization showed two types, the first one is the most numerous and were used as substrate for all identified colours, except for pure black. In fact, fragments that only presented the black pigment, sometimes with lines in white, have been identified on the intonaco layers with ceramic. This remains probably corresponded with a prominent Roman urban villa placed in the Eriteia island of Gades, confirming the importance that this city had within the Roman Empire.

Acknowledgements: This study was financially supported by the Research Project TED2021-132417A-I00 founded by MCIN/AEI /10.13039/501100011033 and by the European Union NextGenerationEU/PRTR, and the Research Project “La gestión de los residuos sólidos en Gades. Aproximación a la caracterización tipológica de los vertidos y su inserción en el entramado urbano de una ciudad costera” (CEIJ-006) Fundación CEiMAR.

How to cite: Domínguez-Bella, S., Lara Medina, M., Pascual Sanchez, M. A., and Molina-Piernas, E.: Archaeometrical characterization of the Roman wall paintings from Gades (Cádiz, Spain)., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20444, https://doi.org/10.5194/egusphere-egu25-20444, 2025.

EGU25-20560 | Orals | ERE1.3

The use of ultrasonic pulse-echo tomography to assess UPV in soft calcarenitic stones 

Emilia Vasanelli, Davide Di Gennaro, Matteo Sticchi, Gianni Blasi, and Maria Antonietta Aiello

Measuring the ultrasonic pulse velocity of stone ashlars belonging to masonry structures provides useful indications for assessing the materials' strength and state of conservation, the need for their possible substitution, and the effectiveness of consolidating treatments. Ultrasound techniques as nondestructive tests preserve the integrity of masonry buildings that especially in Italy often have a cultural and historical-artistic value.
Several correlations linking ultrasonic velocity with the compressive strength of stone materials are available in the literature. These correlations are often developed in the laboratory using small-size samples, high measurement frequencies, and direct transmission measurement modes. In situ, it is often difficult to make measurements under such conditions due to the inaccessibility of both the surfaces of materials and the higher dimension of the elements to investigate. In addition, material surfaces are often affected by deterioration which causes problems in the transducer coupling with measurement surfaces. Furthermore, the use of coupling agents is usually forbidden in the case of artistic artifacts. The ultrasonic tomograph with pulse-echo technology (PE UT) overcomes such difficulties. Pulse-echo method introduces a stress pulse by a transmitter into an object at an accessible surface. The pulse propagates into the test object and is reflected by flaws or interfaces. The surface response caused by the arrival of reflected waves, or echoes, is monitored by receivers. Tomography gives visualization, either by cross-section or 3D images, of the interior structure of the object to find anomalies and determine the material physical properties. PE UT has an array of dry-point contact transducers (DPCT) that enable ultrasonic measurements on rough surfaces without coupling gel, reducing the measuring time and test invasiveness. PE UT employs transverse S-waves instead of longitudinal P-waves because they give more reliable results for degraded materials and in the presence of defects. In the literature, there are several studies in which tomographic images were used to detect the presence of defects in concrete and rock members. In these cases, a reference value of UPV is assumed. On the contrary, few studies use PE UT images to determine UPV on concrete or stone members. Thus, the appropriateness of this technique to assess UPV is still under research due to the lack of a sufficient number of published experimental studies.
In the present paper, the reliability of PE UT in determining the ultrasonic velocity of soft calcarenitic stone elements, known as Lecce stone, is investigated. The measurements are compared with those conducted with conventional transducers at different frequencies in direct and indirect modes. The measurements are also carried out considering the presence of water in the material, which strongly influences not only the ultrasonic measurements but also the strength of the material itself. Four levels of saturation from dry to fully saturated states are considered. The results of the experimental campaign evidence that PE UT is a reliable technique for UPV assessment, allowing rapid one-side measurements on surfaces in different conditions.

How to cite: Vasanelli, E., Di Gennaro, D., Sticchi, M., Blasi, G., and Aiello, M. A.: The use of ultrasonic pulse-echo tomography to assess UPV in soft calcarenitic stones, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20560, https://doi.org/10.5194/egusphere-egu25-20560, 2025.

In the realm of railway infrastructure, the safety of railway road base structures is of paramount importance. A conventional railway raod base is composed of three distinct layers: square cement sleepers positioned at the top, ballast situated in the middle, and undisturbed bedrock or soil at the base. Railway roadbase are prone to a variety of structural challenges that can manifest differently based on their geographical context. In excavated railway sections, particularly those located in limestone regions, the occurrence of karst cracks and cave formations is a significant concern. Such geological phenomena may lead to the ballast stones falling into underlying cavities, thereby diminishing the thickness of the ballast layer. This reduction can adversely affect the bearing capacity of the railway sleepers, thereby compromising safety during train operations. Additionally, during the summer months, ballast may become saturated with rainwater, resulting in the formation of mud and mud overflow to the ground surface; conversely, in winter, the volume of ballast may increase due to ice heaving, leading to deformation of the railway track and square cement sleepers. Both scenarios pose safety risks for train operations and necessitate a thorough investigation of the ballast structure with ground penetrating radar.

To assess the condition of the raiway ballast structure, a Ground Penetrating Radar (GPR) system, along with three sets of air coupled antennas operating at a center frequency of 1.0 GHz, was employed. The antennas were strategically positioned at the front of the train, elevated 45 cm above the square cement sleepers, and arranged on the left, center, and right sides of the railway track. The GPR system successfully detected the railway cement sleepers and ballast structures, producing a two dimensional longitudinal profile for each antenna. The hyperbolic reflections generated by the cement sleepers were pronounced, which interfered with the emitted signals from the ballast, obscuring the ballast interface. Data processing was performed using a specialized local removal curve algorithm, which utilized a raw profile to subtract the local curve profile of the square cement sleepers, thereby eliminating the influence of the square cement sleepers. This data processing procedure resulted in a continuous reflection signal from the ballast layers, allowing for the identification of water distribution in water-bearing areas, variations in ballast thickness, and the structural characteristics of the railway subgrade and ballast layers in limestone regions. The Ground Penetrating Radar equipped with a horn antenna was utilized for scanning the railway ballast, yielding ballast clear reflection signals when combined with the specialized local removal curve method, thereby enhancing railway safety.

How to cite: Deng, X.: The method to get clear image for the railway ballast structure with the Ground Penetrating Radar Horn Antenna, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1404, https://doi.org/10.5194/egusphere-egu25-1404, 2025.

EGU25-1815 | ECS | Orals | ERE1.7

Electromagnetic coupling analysis and removal in large-depth induced polarization method by using the relative phase 

Haojie Qin, Rujun Chen, Zhenxing Ji, and Qunagong Wang

As shallow mineral resources continue to deplete, deep mineral exploration has emerged as an essential trend in the mining industry. One of the most direct and effective methods to enhance exploration depth is by increasing the spacing of the current electrode in the array. However, this increase often results in a stronger electromagnetic (EM) coupling effect, which can significantly interfere with the induced polarization (IP) signal. To address these challenges, this paper calculates the EM coupling effects of various measuring arrays in both uniform half-space and layered media using analytical methods. Based on these calculations, we further analyze the impact of various factors on the intensity of EM-coupling interference in the layered media model, including the type of measuring array, the spacing of the current-electrodes, as well as the resistivity and frequency. Ultimately, based on the differences in the phases of the IP and the EM-coupling in the frequency domain, we derive the calculation formula of the relative phase method and analyze its decoupling effect at various application scenarios. The results indicate that an increase in the spacing of the current electrode, a decrease in ground resistivity and an increase in working frequency will significantly enhance the intensity of EM coupling interference. Under consistent conditions and detection depths, the EM coupling interference is typically greater for Schlumberger array compared to pole-dipole array. By employing the relative phase method, the biggest working frequency of the pole-dipole array can be enhanced by a factor of four, while the Schlumberger array can experience an increase of 10 to 11 times. It demonstrates that the relative phase method has a certain effect for removing the EM-coupling in large-depth IP exploration. The research provides significant guidance for the field implementation of large-depth IP exploration.

How to cite: Qin, H., Chen, R., Ji, Z., and Wang, Q.: Electromagnetic coupling analysis and removal in large-depth induced polarization method by using the relative phase, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1815, https://doi.org/10.5194/egusphere-egu25-1815, 2025.

The definition of apparent resistivity is a critical aspect of in electromagnetic methods, particularly in the context of the electrical source transient electromagnetic method (ESTEM), which has not been well resolved. This study presents a novel concept termed pulse impedance for ESTEM, which is defined as the ratio of the first-order time derivative (pulse response) of the horizontal electric field to the vertical magnetic field. This innovative definition facilitates the derivation of a clear and explicit expression for apparent resistivity that maintains accuracy across the entire range of periods. The pulse impedance approach notably eliminates the source term from the calculations, resulting in an apparent resistivity that is independent of source parameters, thus enhancing the robustness and reliability of the resistivity estimations. The efficacy of this approach was corroborated through the analysis of data obtained from both numerical simulations and field measurements.

How to cite: Chen, W. and Zhu, Y.: Pulse Impedance: A New Approach to Defining Apparent Resistivity of Electrical Source Transient Electromagnetic Data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1844, https://doi.org/10.5194/egusphere-egu25-1844, 2025.

EGU25-1868 | ECS | Posters on site | ERE1.7

Lithology identification method based on Multi-mode adaptive prediction system: Algorithms and Applications 

Pengfei Lv, Guoqiang Xue, and Weiying Chen

Lithology identification is crucial in mineral and energy resource exploration as it determines geological composition and guides exploration activities, improving resource location and evaluation efficiency. The advancement of artificial intelligence technology has promoted the application of machine learning-based multi-source geophysical data fusion methods in lithology identification. However, due to the differences in geophysical exploration techniques and data types across mining areas, single machine learning methods often struggle to adapt to diverse geological environments, lacking necessary universality and robustness, which severely restricts the practical application of intelligent identification technology in actual exploration. To address these limitations, this study introduces a Multi-mode Adaptive Prediction System (MAPS) for lithology identification. MAPS innovatively integrates three learning models (supervised, semi-supervised, and unsupervised learning), and can automatically select the most suitable learning mode based on prior information such as the quantity and quality of existing labeled samples and the completeness of geological background information, achieving rapid and accurate lithology identification. We verified MAPS's performance advantages through extensive comparative experiments: in supervised learning mode, compared to Support Vector Machine (SVM) and Naive Bayes classifier, accuracy improved by 0.7% and 3.5% respectively, with F1 scores increasing by 3.4% and 4.5%; in semi-supervised learning mode, compared to semi-supervised fuzzy C-means algorithm and self-learning algorithm, accuracy and F1 scores improved by a minimum of 33.67% and 0.15 respectively; in unsupervised mode, compared to traditional fuzzy C-means and Gaussian mixture models, MAPS demonstrated superior ability to mine and construct internal data structures, showing stronger feature learning capabilities. Furthermore, MAPS has shown excellent performance in the practical application of coal seam location prediction. The coal seam locations predicted by the system are highly consistent with actual drilling results, further validating MAPS's significant application potential in practical engineering. In conclusion, MAPS significantly improves the efficiency and accuracy of lithology identification, providing reliable technical support for mineral and energy resource exploration with broad application prospects.

 

 

How to cite: Lv, P., Xue, G., and Chen, W.: Lithology identification method based on Multi-mode adaptive prediction system: Algorithms and Applications, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1868, https://doi.org/10.5194/egusphere-egu25-1868, 2025.

EGU25-2763 | ECS | Orals | ERE1.7

Integrated MT, Gravity, and Seismic Inversion and Interpretation for Improved Subsurface Imaging 

Xiaolei Tu, Adam Schultz, and Qingyun Di

We present a comprehensive geophysical methodology that combines magnetotelluric (MT), gravity and/or seismic data in a joint 3-D inversion framework to reduce interpretational uncertainty and provide a more accurate subsurface image of volcanic and geothermal systems. The methodology leverages the complementary sensitivities of each dataset—electromagnetic data for electrical conductivity, gravity for density contrasts, and seismic for velocity variations—to characterize subsurface structures more robustly than any single method alone.

As a demonstration, we apply this integrated workflow to Newberry Volcano in central Oregon, an important target for geothermal development and Enhanced Geothermal System (EGS) research. Broadband MT and gravity data were inverted jointly and integrated with existing seismic models. The integrated inversion/interpretation confirms a prominent conductive feature beneath the volcano’s southern rim and flank (SRFF), which is also marked by low density and slower seismic velocities. This feature extends from the southern caldera floor near the 1,300-year-old Big Obsidian Flow (BOF) to depths beyond 4 km, yet remains disconnected from the sub-caldera magma body.

Through this Newberry Volcano example, we illustrate how a multi-parameter approach provides improved resolution of the subsurface architecture and fluid flow pathways, highlighting the critical role of joint inversion in unraveling complex volcanic systems. The results not only shed light on Newberry’s hydrothermal alteration and fluid pathways but also underscore the broader applicability of our integrated methodology in guiding geothermal exploration and de-risking subsurface resource assessments.

How to cite: Tu, X., Schultz, A., and Di, Q.: Integrated MT, Gravity, and Seismic Inversion and Interpretation for Improved Subsurface Imaging, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2763, https://doi.org/10.5194/egusphere-egu25-2763, 2025.

Thrust fault zones around the Tibetan Plateau (TP) record the tectonic evolution between the Plateau and its surrounding terranes, which is helpful for understanding the uplift mechanism and deformational processes of the TP. The Longmenshan fault (LMSF) is the tectonic boundary (TB) between the Yangtze terrane (YT) and Songpan-Garze terrane (SGT), while the TB of its western segment, either the Lijiang-Xiaojinhe fault (LXF) or Jinhe-Qinghe fault (JQF), is controversial. Therefore, we conducted magnetotelluric (MT) imaging, surface structure surveys, and petrologic analysis to further determine the deep–shallow structural relationship of the western LMSF segment. Resistors R1 and R2 revealed by MT imaging may have originated from different magmatism. Among them, R2 may have originated from plume underplating, which is consistent with previous studies, while R1 may have originated from the residue of episodic mafic magma intrusion along the JQF over a broader period. Based on regional geophysics, surface structural patterns and petrologic mineralogy, it is suggested that the JQF may have deformed deep into the lower crust or upper mantle, accommodating the southeast expansion of the TP by thrusting and acting as the TB between the YT and SGT before ~15 Ma. After ~15 Ma, due to the activation of the large-scale strike-slip faults, the LXF gradually replaced the JQF to dominate the structural deformation of the western LMSF segment. Our results indicate that the above tectonic transition might be associated with the geodynamic process from centralized deformation to diffuse deformation within the southeast TP during the late Cenozoic.

How to cite: Qiao, W., Jian, Y., Shibin, X., and Guozhong, L.: Cenozoic tectonic transition within the western segment of theLongmenshan fault, southeast margin of the Tibetan Plateau: Insights fromgeological and geophysical data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3388, https://doi.org/10.5194/egusphere-egu25-3388, 2025.

In the past decades, electromagnetic (EM) logging while drilling (LWD) has been widely used for well landing and geosteering in high angle and horizontal wells. Recently, this technology has been extended to geo-stopping applications in vertical wells and deviated wells, leveraging its excellent look-ahead-of-bit capability, particularly in ultra-deep reservoirs. Compared to traditional look-around applications in horizontal wells, achieving look-ahead capability is significantly more challenging because the sensitive region of the tool's response is primarily concentrated in the formation between the transmitting and receiving coils. Current look-ahead methods typically use the information from the drilled formation as a constraint to invert the formation ahead of the bit. However, this approach heavily relies on the accuracy of the surrounding formation property measurements. Therefore, to enhance the look-ahead capability and accuracy, it is necessary to further improve the contribution of the formation ahead of the bit to the tool's response.

In this paper, we analyze the spatial sensitivity of the magnetic field components based on the Born geometric factor. Among these, the coaxial (Hzz) and coplanar (Hxx and Hyy) components exhibit look-ahead sensitivity and can be used for look-ahead detection. In EM LWD look-ahead measurements, it is common to combine the coaxial and coplanar components to define the look-ahead signal. We further derive the spatial sensitivity functions for phase shift and amplitude ratio, with results showing that the primary contribution to the look-ahead signal still comes from the formation between the transmitter and receiver. To address this, we propose a signal enhancement method based on Multi-TR-spacing signal superposition. By exploiting the differences in sensitivity ranges of signals from different TR spacings, the method optimizes the sensitive space through signal superposition, thereby improving the tool’s look-ahead performance. Finally, we employ numerical simulation algorithms to compare the look-ahead capability of the new method with traditional methods. Simulation results demonstrate that, the look-ahead signal obtained with the new method is significantly enhanced to 1.5 times, and the maximum distance range has been increased by 30% that enabling the detection of interfaces at greater distances. Additionally, the new method results in a stronger sensitivity to the formation boundaries ahead of the bit, suggesting an improvement in inversion accuracy. It is important to emphasize that the method proposed in this paper can also be extended to look-around detection, for further enhancing the sensitivity of a specific detection area.

How to cite: Liao, X., Wu, Z., and Yue, X.: Sensitivity Analysis and Optimization for Enhancing the Look-Ahead Capability of Electromagnetic Logging While Drilling Tools, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5673, https://doi.org/10.5194/egusphere-egu25-5673, 2025.

The semi-airborne transient electromagnetic (SATEM) method has attracted increasing attention for its efficiency in various exploration scenarios. A recent geophysical survey in northern Gansu, China, employed the SATEM system to investigate the potential distribution of Volcanogenic Massive Sulfide (VMS) deposits. Several observed data profiles showcase significant late-time negative values, which were attributed to induced polarization (IP) effects associated with VMS minerals, as prior time-domain IP (TDIP) measurements revealed their high polarizability characteristic in such regions. More recently, interest in interpreting TEM data with IP effects has notably increased in the geophysical community as these effects can significantly disturb the data, leading to misinterpretation using the conventional resistivity-only (RO) inversion approach. Guided by the Cole-Cole model, which quantitatively describes the IP effect of materials using DC resistivity and other three IP parameters, numerous previous inversion studies have been successfully conducted to extract multiparametric information.

In this work, one field data profile is demonstrated in Figure. 1a and was inverted using a quasi-2D hybrid constrained inversion algorithm including three terms: (1). The classical data misfit functional; (2). Laterally smoothing regularization; (3). Fuzzy c-means (FCM) clustering regularization, which can facilitate the integration of the prior geophysical information. Local geological investigations suggest that VMS targets are primarily deposited in intact fracture spaces, which offer favorable conditions for mineralization and storage. The inversion results, shown in Figure. 1b, display clearly high-to-moderate resistivity interfaces surrounded by distinct IP value distributions. Moreover, the extending high IP distribution toward the deep is supposed to result from mineral dissemination, resulting in high resistive polarization anomalies and deeper conductive polarization anomalies caused by mineral enrichment. The above characteristics are considered the indicators of VMS minerals in such area.

To sum up, the IP-incorporated inversion facilitates the interpretation of TEM data collected over high polarization areas. However, the serious ill-pondness issue of multiparametric inversion brings a great challenge to result reliability, which largely depends on the selection of the starting model and inversion scheme. Integrating the geological and geophysical information in the inversion offers a promising way to avoid misinterpretation

How to cite: Lu, J., Wang, X., Guo, M., and Xue, S.: Application of the semi-airborne transient electromagnetic method over the VMS deposit and data interpretation incorporating induced polarization effects, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7917, https://doi.org/10.5194/egusphere-egu25-7917, 2025.

EGU25-8112 | Orals | ERE1.7

Experimental Study on the Induced Polarization of Carbonate Rocks 

Ming Ma, Jianguo Zhao, Bohong Yan, Yu Zhang, Yangyang Sun, and Fang Ouyang

The induced polarization (IP) parameters, such as the peak relaxation time and polarizability, have the potential to characterize pore structures of geomaterials and can be further used to distinguish lithology. However, the systematic experimental research on the IP response of carbonate rocks is scarce. To fill this gap of knowledge, we investigated the complex resistivity of 16 carbonate rocks, including dolostone and limestone, and discussed the applicability of existing induced polarization mechanisms for carbonate rocks. The relationship between IP parameters and pore structures were further analyzed by the experiment on variable confining pressure. The results indicate that the carbonate rocks with intergranular micropores or microfractures exhibit observable induced polarization response, where the amplitude and phase of complex resistivity are frequency-dependent, and still exist under high pressure conditions. Dolostone is characterized by low resistivity, high peak relaxation time, low polarizability, and the bell-shaped phase spectrum. Moreover, Stern layer polarization can explain the positive correlation relationship between peak relaxation time and pore size in samples with intercrystalline micropores. In contrast, membrane polarization provides a mechanism for the larger peak relaxation time in samples with microfractures, which is related to the low pore aspect ratio.

How to cite: Ma, M., Zhao, J., Yan, B., Zhang, Y., Sun, Y., and Ouyang, F.: Experimental Study on the Induced Polarization of Carbonate Rocks, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8112, https://doi.org/10.5194/egusphere-egu25-8112, 2025.

EGU25-8531 | ECS | Posters on site | ERE1.7

DC resistivity surveys compared to direct 3D surveys methods to characterize underground cavities in eastern Sicily (Italy) 

Gabriele Morreale, Sabrina Grassi, Danilo Messina, Pietro Monforte, Gaetano Giudice, Gabriele Quattrocchi, and Sebastiano Imposa

The study and characterization of caves is a complex problem because not all underground cavities are accessible and therefore cannot be characterized by direct methods, such as topographical or geomatic methods. Therefore, geophysical surveys play a key role, as they can provide information on the size and shape of underground cavities from surface measurements.

In this work, two underground cavities characterized by different geological contexts and located in eastern Sicily (Italy) were studied: i) the “Micio Conti Lava tube”, a lava cave located in the municipality of San Gregorio di Catania and ii) the “Chiusazza Cave”, a complex karst cave located in the area of Syracuse. The two caves were investigated using both DC resistivity surveys and direct methods for 3D reconstruction (terrestrial laser scanner (TLS) and photogrammetry by unmanned aerial vehicle (UAV)).

In the “Micio Conti Lava tube”, N. 11 ERT (electrical resistivity tomography) profiles and N. 18 TLS stations were performed, while in the “Chiusazza cave”, N. 11 ERT profiles and N. 23 TLS stations were implemented.

In both cases, aerophotogrammetry was used to generate the 3D models of the epigeal environments. Geoelectrical surveys were performed using the dipole-dipole quadripolar configuration and a cluster analysis (K-means) was performed on the 3D resistivity models of both caves. This analysis revealed for each site two groups of clusters, highlighting areas with different resistivity values. A comparison between the resistivity models and the clusters showed a good overlap between the clusters identified in the central portion of the two models and the areas characterized by the highest resistivity values. This approach allowed the identification of isosurfaces for both areas that enclose the areas associated with the shape, position and size of the investigated cavities. In the "Micio Conti Lava Tube" area, the cavity is characterized by resistivity values higher than 17000 Ω-m while, in the Chiusazza cave area, the cavity is identified by resistivity values higher than 4000 Ω-m.

Comparing the results obtained by resistivity and 3D TLS models, an excellent correspondence can be observed for the "Micio Conti lava tube". Instead, for the "Chiusazza Cave", the models do not seem to fit perfectly in the central portion, probably due to the limited coverage of geoelectrical surveys in this area due to the prohibitive logistic conditions of the site.

This study confirms that DC resistivity methods are suitable for identifying and characterizing underground cavities in different geological contexts. Cluster analysis allowed to identify the isosurface value to be assigned as the boundary of the area of ​​the studied cavities. The results of this study clearly show that by integrating geophysical and 3D survey techniques, it is possible to increase the mapping and understanding capabilities of these geological structures, even if they are inaccessible from the surface.

How to cite: Morreale, G., Grassi, S., Messina, D., Monforte, P., Giudice, G., Quattrocchi, G., and Imposa, S.: DC resistivity surveys compared to direct 3D surveys methods to characterize underground cavities in eastern Sicily (Italy), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8531, https://doi.org/10.5194/egusphere-egu25-8531, 2025.

EGU25-8667 | ECS | Posters on site | ERE1.7

An electromagnetic investigation of the continent-ocean transition southwest of the UK. 

Yuan Li, Kyle Ivey, Steven Constable, Tim Minshull, and Gaye Bayrakci

In ocean-continent transition zones at rifted continental margins, distinguishing between crustal rocks, hydrated mantle rocks, and the boundary between continental and oceanic mantle is crucial. These materials exhibit distinct resistivity characteristics, making them identifiable through geophysical techniques. Marine Controlled-Source Electromagnetic (CSEM) surveys are particularly effective in mapping subsurface structures both onshore and offshore due to their sensitivity to conductivity contrasts.

Our study focuses on using multiple geophysical techniques to investigate crustal and mantle rocks at magma-poor rifted margins. We focus on the continent-ocean transition at the Goban Spur, located southwest of the UK. Here, previous seismic work suggested the presence of a broad zone of exhumed serpentinised mantle, in between continental crust confirmed by drilling and oceanic crust represented by the prominent linear seafloor spreading magnetic anomaly 34. We deployed 49 seafloor instruments on a c. 200 km transect spanning these three basement types, coincident with a pre-existing high-quality seismic reflection profile, to collect seismic, magnetotelluric (MT), and controlled-source electromagnetic data.

For navigation, the CSEM system integrated USBL positioning, CTD measurements, and an altimeter. The transmitter utilized a compact waveform with a fundamental frequency of 0.25 Hz, enhanced by maximizing the amplitude of the 3rd and 7th harmonics. The transmitter dipole moment was 30,000 A·m, powered by a current of 100 A.

For data analysis, the compact waveform was processed in short 4-second time windows. We do stack the 4-second FFT up to 60 seconds or longer.  This approach retained essential information while enhancing the signal-to-noise ratio, enabling robust time-series analysis.

CSEM and MT methods have shown promise in resolving debates about lithospheric structure. While these techniques have previously imaged fluid-rich zones in subduction settings, this study is the first to apply them to continent-ocean transitions in rifted margins. We present results from preliminary analysis of both CSEM and MT datasets, focusing on lateral changes in resistivity at the seaward limit of continental crust.

How to cite: Li, Y., Ivey, K., Constable, S., Minshull, T., and Bayrakci, G.: An electromagnetic investigation of the continent-ocean transition southwest of the UK., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8667, https://doi.org/10.5194/egusphere-egu25-8667, 2025.

EGU25-14126 | ECS | Orals | ERE1.7

3-D modeling of coupled geophysical fields for hidden hazards in the embankment dam using YOLO convolutional network model 

Hui Yu, Songtao Hu, Shangfu He, Hui Chen, Juzhi Deng, and Shuo Wang

Geophysical techniques are an efficient method for identifying hidden hazards in embankment dams due to the presence of significant physical differences in dam hazards. However, there is still a lack of sufficient understanding of the coupling relationship between different geophysical fields of different hazards, which hinders the detection accuracy of geophysical methods. By combining the theories of seepage field, stable electric field, electromagnetic wave field, and elastic wave field, a multi-physics coupling equation and boundary conditions for the hidden hazard model of embankment dams are established. Based on different geophysical methods, the geophysical responses of dam models with different water levels, hazard types, and sizes were modeled and used as the library of training samples. These samples were thoroughly trained using the YOLO convolutional network model, and training metrics like recall, accuracy, and loss curve were used to assess the quality. The results indicate that the GPR and seismic images are more accurate in identifying the hazard of the cavity, ant nest, and fracture, whereas the ERT is more successful in identifying the leakage risks. In addition, the location of the submerged surface can be accurately determined by the ERT, which is more sensitive to the water level.

 

This work was funded by the Science and Technology Project of Jiangxi Province (2022SKLS04, 2023KSG01008) and the National Natural Science Foundation of China (42374097)

How to cite: Yu, H., Hu, S., He, S., Chen, H., Deng, J., and Wang, S.: 3-D modeling of coupled geophysical fields for hidden hazards in the embankment dam using YOLO convolutional network model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14126, https://doi.org/10.5194/egusphere-egu25-14126, 2025.

EGU25-14405 | ECS | Orals | ERE1.7

Research on localization technology for dam leakage channels based on coupled electric and magnetic fields 

Suiming Liu, Hui Chen, Juzhi Deng, Shangfu He, Shuo Wang, and Yufeng Chen

Based on the mechanism of current density formation under natural electric fields and artificial stable current sources, this study proposes a multi-physics coupling theory involving seepage fields, ion diffusion fields, and stable electric fields induced by leakage. Coupling equations and boundary conditions for electric and magnetic fields were formulated based on fundamental laws of Ohm’s law and Biot–Savart law. A finite element-infinite element numerical simulation method was used to achieve three-dimensional response characteristics of coupled electric and magnetic fields in embankment leakage scenarios by incorporating conversion relationships for the water content, resistivity, and ion concentration. Based on the distribution characteristics of coupled electric and magnetic fields, a detection technique for locating leakage channels in embankment dam was proposed. This technique enhances leakage channel signals by applying an artificial stable electric field on both upstream and downstream sides of the channel. Subsequently, precise localization of leakage risks is achieved by observing two components of the coupled electric field or three components of the magnetic field on the dam surface. This new method was applied to locate the leakage channel at a pond in Hangzhou. The detection results have been validated by the drilling results, which demonstrated that this technique offers higher precision and better detection performance compared to traditional high-density resistivity methods. This work validate the effectiveness of the coupled electric and magnetic field-based detection method and provide a novel solution for embankment leakage detection.

How to cite: Liu, S., Chen, H., Deng, J., He, S., Wang, S., and Chen, Y.: Research on localization technology for dam leakage channels based on coupled electric and magnetic fields, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14405, https://doi.org/10.5194/egusphere-egu25-14405, 2025.

EGU25-14411 | ECS | Posters on site | ERE1.7

Field study on the application of time-lapse electrical resistivity tomography to assess the performance of an inclined multi-layer cover system reducing water infiltration 

Leila Bedoui, Adrien Dimech, Vincent Boulanger-Martel, Bruno Bussière, Karine Sylvain, Thierry Impinna, and Benoît Plante

Post-mining can raise environmental issues, including water contamination in tailings storage facilities. Contaminated mine drainage can occur in these facilities when oxygen and water come into contact with tailings containing sulfides. In the past 20 years, various reclamation methods have proven to be effective in preventing potential contamination, such as the use of multi-layer cover systems. These engineered covers consist of successive layers with different hydrogeological properties to prevent water from reaching tailings. One way of assessing the effectiveness of these covers on the field is to monitor the flow of water within the cover over time, using time lapse electrical resistivity tomography (TL-ERT) in conjunction with hydrogeological instruments. This method allows to recover the spatio-temporal distribution of the soil electrical conductivity, and thus providing an image of the water flow in the near subsurface.

The objective of this project is to monitor water flow within a mine cover system which acts as a barrier to water infiltration into tailings using TL-ERT. This approach involves the use of numerical models, combined with field and laboratory data processing.

This study presents preliminary results from the two-weeks field campaign that was conducted in Fall 2024 at a tailing storage facility in Quebec where a multi-layer cover system is installed on a 7% slope. The cover configuration consists of four layers: 30 cm of silt, 20 cm of gravel, 30 cm of moisture-retaining silt, and 20 cm of gravel as a capillary break (from top to bottom). A 32 m-long ERT profile was installed along the slope of this cover with 64 electrodes and a spacing of 0.5 m. A 20 cm-high, 30 cm-wide and 2.75 m-long trench was excavated perpendicularly to the ERT profile, one-third along the profile. An infiltration test was performed, during which a total of 2000 L of a 1000 μS/cm saline tracer was injected into the trench over a period of 4 hours. TL-ERT monitoring consisted of acquiring a dataset of 65 ERT images using the Wenner configuration, every hour during the infiltration test, and every 6 hours thereafter for a week.

Preliminary results from field data inversion showed a spatio-temporal variation in resistivity associated with the start of the infiltration test. Near the trench, the inverted conductivity increased by a factor of two soon after the start of the injection, and a slightly conductive bulb appeared along the slope in the hours following the test. In addition, over the course of the two-week recording period, the surface of the cover became increasingly resistive, which can be associated to a significant drop in temperature between the beginning and end of the monitoring period (no rain was monitored during the monitoring period). The future steps of the processing will include a temperature correction to ensure that resistivity variations are only attributed to water inflow. Finally, thermo-hydrogeological modeling of the multilayer cover system during the infiltration test will allow to compare the geophysical results with modeled water dynamics.

How to cite: Bedoui, L., Dimech, A., Boulanger-Martel, V., Bussière, B., Sylvain, K., Impinna, T., and Plante, B.: Field study on the application of time-lapse electrical resistivity tomography to assess the performance of an inclined multi-layer cover system reducing water infiltration, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14411, https://doi.org/10.5194/egusphere-egu25-14411, 2025.

EGU25-14438 | ECS | Orals | ERE1.7

A New Compensated Design of Deep-reading Look-ahead Method in Electromagnetic Logging-while-drilling 

Yanxue Wang, Lei Wang, Yiren Fan, Xinmin Ge, Xizhou Yue, and Tianlin Liu

With the intensifying exploration and development of deep and unconventional oil and gas reservoirs, the advanced prediction of the formations during drilling plays a pivotal role in mitigating drilling risks and optimizing drilling parameters. This technique serves as a crucial foundation for enhancing drilling trajectory accuracy and reducing operational costs. Currently, ultra-long spacing and low-frequency technologies enable the look-ahead, ultra-deep electromagnetic (EM) logging-while-drilling (LWD) tool to detect the top of the target formation more than 30 meters ahead of the bit. However, the measurement signal is predominantly influenced by the stratigraphy surrounding the instrument, resulting in a very low proportion of the spatial contribution in front of the bit. Consequently, the inversion process, which is integral to look-ahead detection, poses challenges for real-time geosteering.

To tackle this challenge, this study introduces a novel multi-spacing interleaved compensating antenna design aimed at augmenting the electromagnetic scattering field signal share at the forward stratigraphic interface. The spatial distribution of the new look-ahead detection signal is characterized using geometric factor theory. Additionally, the response characteristics and look-ahead detection capability of the proposed scheme are simulated and analyzed based on a response fast forwarding algorithm. The integral geometry factor associated with the novel look-ahead measurement effectively excludes contributions from the stratigraphy in the vicinity of the instrument, thereby enhancing the proportion of the look-ahead signal. This advancement is particularly beneficial for look-ahead detection. Simulations based on a single interface model reveal that the response diminishes to zero when the instrument is positioned at a considerable distance from the interface, whereas it attains non-zero values as the tool approaches the interface. In addition, the polarity of the response depends on the difference in resistivity between the two sides of the interface, which offers a more intuitive interpretation compared to existing methodologies. Furthermore, variations in magnetic field attenuation across different spacings leveraged to optimize spacing and signal synthesis combinations, further bolstering the capability of look-ahead detection. Numerical results demonstrate that the new method significantly improves the look-ahead detection capability of phase difference measurements compared to existing methods, with a maximum look-ahead depth of detection (DOD) increased by approximately 50%. The look-ahead DOD of amplitude ratio signal is comparable to that of existing methods.

In summary, the proposed method provides a more intuitive response to resistivity anomalies ahead of the bit, reducing the update time for forward geostructural information and enabling improved look-ahead detection. This innovation will provide a more cost-effective drilling solution for proactive risk avoidance in straight or low-angle wells and optimize casing shoe placement and coring operations.

How to cite: Wang, Y., Wang, L., Fan, Y., Ge, X., Yue, X., and Liu, T.: A New Compensated Design of Deep-reading Look-ahead Method in Electromagnetic Logging-while-drilling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14438, https://doi.org/10.5194/egusphere-egu25-14438, 2025.

EGU25-19846 | ECS | Posters on site | ERE1.7

Geophysical Studies of Electrometry and GPR for Mapping Underground Pollution Spread Around the Petromidia Navodari Refinery 

Andrei Gabriel Dragos, Sorin Anghel, Gabriel Iordache, Bogdan Baraitareanu, and Alexandra-Constanța Dudu

The rapid growth of the oil and gas industry, driven by the increasing demand for fossil fuels, has led to significant environmental challenges. Among these, hydrocarbon pollution around refineries has emerged as a critical issue that was largely overlooked until recent decades. Romania, a prominent player in the petroleum sector, continues to rely on substantial reserves for fuel production. However, the environmental consequences of refining and transporting petroleum products were historically ignored, leading to widespread soil and groundwater contamination.This study focuses on the Petromidia Navodari Refinery, one of Romania’s most important refineries, and investigates the extent and impact of underground hydrocarbon pollution. To achieve this, geophysical methods such as electrometry and Ground Penetrating Radar (GPR) were employed alongside soil drilling for sample analysis. The investigation covered several zones, each spanning 400 to 600 square meters, and extended over several kilometers surrounding the refinery. Measurements reached depths of up to four meters, encompassing the water table—a critical layer for environmental and public health.

Electrometric data revealed high resistivity values at depths of 0.5 to 3 meters, indicating the presence of hydrocarbons, which impede electrical conductivity. These findings align with the depth of the groundwater table, highlighting the risk of pollutant transport through underground water systems to populated areas. GPR surveys identified anomalies at depths of 1 to 2.5 meters, corresponding to zones affected by hydrocarbon infiltration. The integration of GPR and electrometric data with soil sample analyses confirmed hydrocarbon contamination in these layers.

Using these datasets, a detailed map was created to illustrate the spread of underground pollution, revealing both the affected area and the dynamic movement of contaminants. Additional mapping of groundwater flow patterns allowed for the estimation of the speed and direction of hydrocarbon migration, enabling predictions of the contamination’s future expansion.

This research underscores the significant environmental impact of petroleum processing and transport, particularly the contamination of soil and aquifers. Such pollution poses severe risks to public health, agriculture, and ecosystems. By identifying the affected zones and quantifying the extent of contamination, this study provides valuable insights for mitigation strategies.

The findings emphasize the urgent need for stricter environmental policies and remediation measures around refineries. These should include monitoring systems, improved waste management practices, and technologies for reducing hydrocarbon emissions into the environment. The integration of geophysical techniques such as electrometry and GPR proves to be an effective approach for assessing and managing underground pollution.

In conclusion, the study highlights the critical importance of addressing refinery-related pollution through comprehensive assessments and informed interventions. By providing a scientific basis for action, this research supports efforts to mitigate the environmental and public health impacts of the oil and gas industry.

How to cite: Dragos, A. G., Anghel, S., Iordache, G., Baraitareanu, B., and Dudu, A.-C.: Geophysical Studies of Electrometry and GPR for Mapping Underground Pollution Spread Around the Petromidia Navodari Refinery, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19846, https://doi.org/10.5194/egusphere-egu25-19846, 2025.

EGU25-20337 | ECS | Orals | ERE1.7

Geophysical Multimethod Joint Analysis for Assessing Multi-Layer Covers on Mine Tailings at Two Different Scales 

Thierry Impinna, Adrien Dimech, Gabriel Fabien-Ouellet, Bruno Bussiere, Leila Bedoui, and Vincent Boulanger-Martel

Mine tailings storage is a major challenge for the mining industry due to the risks associated with contaminated mine drainage. Tailings can contain sulfides that, when exposed to atmospheric oxygen and precipitation, generate acidity that can spread downstream from tailings storage facilities. To mitigate this issue, the construction of multi-layer cover systems designed to divert infiltrating water from the tailings represents a promising solution. However, such cover systems are susceptible to deteriorate over time, and their effectiveness must therefore be regularly assessed.

Unlike traditional destructive methods, non-invasive geophysical techniques offer a rapid and cost-effective solution for analysing these cover systems. However, each geophysical technique has its own limitations when used individually. In particular, the ERT-IP (Electrical Resistivity Tomography and Induced Polarization) and MASW (Multi-channel Analysis of Surface Waves) methods can be used to characterize the volumetric properties of soils, such as variations in electrical resistivity and seismic velocities, but often lack the precision to delineate fine interfaces clearly. GPR (Ground Penetrating Radar) and seismic refraction, on the other hand, offer a better resolution for identifying the boundaries between layers but have difficulty in accurately describing the physical properties in volume.

This project aims to demonstrate the potential of a multimethod approach that combines these techniques by jointly analyzing the results to leverage their respective advantages while overcoming individual limitations and biases. Ultimately, the goal is to develop a joint inversion methodology to further refine the imaging of multi-layer cover systems, which are generally shallow and are made from a large range of materials.

This study presents the results from a field campaign conducted on a tailings storage facility where inclined multi-layer cover systems have been constructed to limit water infiltration (~1 m thick). Two longitudinal profiles were analyzed at two different scales. A high-resolution profile (32 m-long, 7% slope), with 64 collocated geophones and electrodes spaced by 50 cm intervals was used to focus on fine-scale variations in the cover layer system. Measurements were taken before, during, and after an infiltration test. A longer profile (100 m-long), with 64 collocated geophones and electrodes spaced by 1 m covered two instrumented sections (a 7% slope and a 28% slope) to provide a larger-scale view and greater depth of investigation. The ERT-IP data (collected using the Wenner protocol) and seismic data were coupled with GPR profiles conducted in continuous mode using 200 MHz and 1500 MHz antennas. All geophysical datasets were surveyed to allow comparison between techniques.

The results are interpreted jointly, in order to exploit the interface detection capabilities of GPR and refraction techniques along with the volumetric characterization provided by ERT and MASW at two different scales, which could improve the applicability of geophysical methods to assess the in situ performance of multi-layer cover systems installed on tailings storage facilities across larger scales.

How to cite: Impinna, T., Dimech, A., Fabien-Ouellet, G., Bussiere, B., Bedoui, L., and Boulanger-Martel, V.: Geophysical Multimethod Joint Analysis for Assessing Multi-Layer Covers on Mine Tailings at Two Different Scales, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20337, https://doi.org/10.5194/egusphere-egu25-20337, 2025.

EGU25-21578 | Posters on site | ERE1.7

Study on the influencing factors of the signal-to-noise ratio of UAV GPR data

Rongyi Qian

EGU25-1710 | ECS | Orals | GD10.1

Fluid flow channeling and mass transport with discontinuous porosity distribution 

Simon Boisserée, Evangelos Moulas, and Markus Bachmayr

The flow of fluids within porous rocks is an important process with numerous applications in Earth sciences. Modeling the compaction-driven fluid flow requires the solution of coupled nonlinear partial differential equations that account for the fluid flow and the solid deformation within the porous medium. Despite the nonlinear relation of porosity and permeability that is commonly encountered, natural data show evidence of channelized fluid flow in rocks that have an overall layered structure. Layers of different rock types routinely have discontinuous hydraulic and mechanical properties.
We present numerical results [1] obtained by a novel space-time method [2] based on a fixed-point scheme inspired by the mathematical analysis [3], combined with a space-time least-squares formulation. This approach can handle discontinuous initial porosity (and hence permeability) distributions. It furthermore exhibits optimal convergence independently of the discontinuities, while standard approximations, as e.g. finite differences, tend to show lower order convergence in discontinuous regimes.
The space-time method enables a straightforward coupling to models of mass transport for trace elements. Our results show the influence of different kinds of layering in the development of fluid-rich channels and mass transport [1].

References
[1] Fluid flow channeling and mass transport with discontinuous porosity distribution, S. Boisserée, E. Moulas and M. Bachmayr, arXiv Preprint (2024), https://doi.org/10.48550/arXiv.2411.14211.
[2] An adaptive space-time method for nonlinear poroviscoelastic flows with discontinuous porosities, M. Bachmayr and S. Boisserée, arXiv Preprint (2024), https://doi.org/10.48550/arXiv.2409.13420.
[3] Analysis of nonlinear poroviscoelastic flows with discontinuous porosities, M. Bachmayr, S. Boisserée and L. M. Kreusser, Nonlinearity (2023), https://doi.org/10.1088/1361-6544/ad0871.

How to cite: Boisserée, S., Moulas, E., and Bachmayr, M.: Fluid flow channeling and mass transport with discontinuous porosity distribution, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1710, https://doi.org/10.5194/egusphere-egu25-1710, 2025.

EGU25-2822 | Posters on site | GD10.1

Optimally accurate operators for partial differential equations 

Nobuaki Fuji and Thibault Duretz
  • In this contribution, we generalise the optimally accurate operators proposed and used in the series of studies on the simulation of seismic wave propagation, especially based on Geller & Takeuchi (1995). Although the operators have been mathematically proven more accurate than conventional methods, the demonstration has been made without a recipe ready for different configurations and the theory is complicated using normal-mode theory, which prevents other physics from applying the methods. Here we show that the operators can be systematically obtained for any form of partial differential equations and we show several applications with numerical examples.

How to cite: Fuji, N. and Duretz, T.: Optimally accurate operators for partial differential equations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2822, https://doi.org/10.5194/egusphere-egu25-2822, 2025.

EGU25-4080 | ECS | Orals | GD10.1

Numerical modeling of simultaneous diffusion and mineral growth 

Annalena Stroh, Pascal Aellig, and Evangelos Moulas

Compositional concentration profiles across individual crystals or diffusion couples are largely determined by diffusion and growth processes. These two processes are particularly important during the formation of high-temperature rocks such as igneous and metamorphic rocks. The numerical simulation of concentration profiles in crystals is a widely used technique in various fields such as geospeedometry or diffusion chronometry. Compared to single crystals, coupled diffusion pairs yield tighter constraints on the experienced temperature and pressure ranges and thus provide additional information for our models. However, the numerical description of concentration profiles within diffusion couples is challenging due to the sharp compositional gradients. Discontinuities in concentration, which are related to the different mineral properties, commonly occur at the interface of two minerals and lead to technical implementation issues.

To address these issues, we have developed a Finite Element (FE) package in Julia that can calculate the evolution of concentration profiles in diffusion couples with moving interfaces. Both growth and diffusion processes are considered. An adaptive grid enables the accurate reproduction of rapid concentration changes and discontinuities. Our code can be applied to various examples of single crystals or diffusion couples, integrating any combination of growth, diffusion, and temperature dependency. Additionally, it is possible to calculate concentration profiles based on the thermodynamically-constrained, Stefan-Interface condition. Results from our models can be used in petrology and geodynamic applications to provide tighter constraints concerning in the pressure and temperature evolution of magmatic and metamorphic mineral assemblages.

How to cite: Stroh, A., Aellig, P., and Moulas, E.: Numerical modeling of simultaneous diffusion and mineral growth, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4080, https://doi.org/10.5194/egusphere-egu25-4080, 2025.

Our previous studies revealed that the impact of small-scale capillary heterogeneities is crucial for accurately predicting carbon dioxide (CO2) plume migration in geological CO2 storage sites, such as the Endurance site in the UK.  While high-fidelity dynamic modelling would require excessive computational resources, conventional upscaling methods of geological models often result in dynamic models underestimating lateral CO2 migrations.

A novel capillary-limit steady-state upscaling approach is based on macroscopic invasion percolation and addresses this accuracy-feasibility trade-off. It incorporates small-scale capillary effects into upscaled local water/gas saturation functions: capillary pressure and phase permeabilities. We are developing an open-source algorithm implementation to encourage industrial adoption of the approach [1]. We present the latest advances in the library's features and performance and numerical experiments on our public set of dynamic models of real CO2 storage sites in the North Sea [2]. 

The latest library advances include substantial parallelisation, single-core optimisations, an optional hydrostatic term, support for anisotropic fine-scale permeability, a stochastic re-upscaling approach for porosity and permeability fields upscaled by averaging, library infrastructure, and more. Numerical experiments aim to assess the impact of upscaling under uncertainties in rock and multiphase flow properties. We also attempt to downscale CO2 plumes simulated at coarse scales using data from the algorithm's percolation step, providing an estimate for fine-scale dynamics.

[1] https://github.com/ImperialCollegeLondon/StrataTrapper
[2] https://github.com/ImperialCollegeLondon/StrataTrapper-models

How to cite: Elizarev, M., Krevor, S., and Muggeridge, A.: Capillary heterogeneity upscaling using macroscopic percolation: code advances and field-scale dynamic CO2 storage simulations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4162, https://doi.org/10.5194/egusphere-egu25-4162, 2025.

EGU25-7270 | Orals | GD10.1

Emulating Viscous Ice Flow Dynamics with Physics-Informed Deep Learning 

Guillaume Jouvet and Guillaume Cordonnier

Modeling the evolution of glaciers and ice sheets over glacial cycle timescales is critical for understanding landscape transformation through glacial erosion, predicting future changes, and assessing their impacts on sea-level rise and water availability. However, solving the partial differential equations (PDEs) governing thermomechanical ice flow at the high spatial and temporal resolutions required for these timescales is computationally prohibitive using traditional CPU-based solvers. GPU-accelerated methods offer a promising pathway to overcome these challenges.
In this study, we present a physics-informed deep learning approach leveraging GPUs, which integrates traditional numerical approximation with deep learning techniques. Using a regular grid and finite difference methods for spatial discretization, we train a Convolutional Neural Network (CNN) to minimize the energy associated with high-order ice flow equations -- a non-linear elliptic problem -- within the iterative time-stepping of a glacier evolution model. The resulting CNN, which is similar to a Variational Physics-Informed Neural Network, delivers multiple benefits: computational efficiency optimized for GPU usage, high fidelity to the original model, unsupervised training that eliminates the need for pre-generated datasets, and relatively simple implementation. Additionally, the emulator incorporates memory of prior solutions, reducing the computational cost of training -- a memory-intensive task.
Embedded within the "Instructed Glacier Model" (IGM) framework, the emulator's capabilities are demonstrated through high-resolution, large-scale simulations of glaciated landscape formation over extended timescales. This work underscores the potential of combining deep learning with physical modeling to develop scalable, efficient tools for simulating complex glaciological processes.

How to cite: Jouvet, G. and Cordonnier, G.: Emulating Viscous Ice Flow Dynamics with Physics-Informed Deep Learning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7270, https://doi.org/10.5194/egusphere-egu25-7270, 2025.

EGU25-9151 | ECS | Posters on site | GD10.1

Scaling staggered grid code on pre-exascale machines 

Iskander Ibragimov, Boris Kaus, and Anton Popov

The transition to exascale (>1000 Petaflops) computing necessitates the adaptation of numerical modeling tools to efficiently utilize emerging high-performance computing architectures. Within the ChEESE-2P project, the further development of LaMEM (Lithosphere and Mantle Evolution Model) focuses on achieving scalable performance on advanced systems, including the EuroHPC supercomputer LUMI (currently #3 in Europe). Taking advantage of using the PETSc library, LaMEM demonstrates strong and weak scalability, achieving linear performance up to 512 compute nodes and supporting high-resolution simulations with grids up to 10243

In response to the increasing emphasis on GPU-based computing, ongoing efforts are directed towards optimizing LaMEM for GPU architectures, including both NVIDIA and AMD systems. Preliminary results highlight significant progress in enabling GPU-accelerated runs and improving resource utilization. This work highlights LaMEM's ability to perform large-scale geodynamic simulations, contributing to the broader goal of integrating physics-based models with available data.

How to cite: Ibragimov, I., Kaus, B., and Popov, A.: Scaling staggered grid code on pre-exascale machines, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9151, https://doi.org/10.5194/egusphere-egu25-9151, 2025.

EGU25-10269 | ECS | Posters on site | GD10.1

Leveraging Differentiable Programming in Julia: Forward and Inversion Modeling of Two-Phase Systems 

Jacob Frasunkiewicz, Boris Kaus, Anton Popov, Christian Schuler, and Nicolas Riel

From complex magmatic systems to geothermal reservoirs, fluid-rock dynamics have posed immense modeling hurdles in the Geosciences for decades. These systems are influenced by interactions between magmatic heat sources, fluid flow, host rock deformation, and chemical heterogeneities. To enhance our understanding and predictive capabilities of these intricate systems, we develop a novel forward and inverse modeling code designed to simulate fluid migration within a deforming, porous host-rock. We employ the Julia programming language, chosen for its differentiability and efficiency, facilitating the simple integration of various composable packages.

Forward simulations are performed in the advanced automatic differentiation (AD) framework of Julia, allowing for flexible adjustments of the underlying coupled system of equations. We utilize a staggered-grid, implicit finite-difference solver, along with the GeoParams.jl package to implement visco-elasto-plastic rheologies and solve the coupled fluid-rock interactions under non-linear Darcy and incompressible Stokes-flow regimes.

The AD framework of Julia allows for the application of the adjoint method in parameter sensitivity analysis, significantly reducing computational demands compared to traditional inversion techniques. This framework lays the foundation for adjoint inversions as the gradients calculated for the sensitivities are needed for gradient descent algorithms. The effectiveness of our framework is demonstrated through representative case studies, illustrating its applicability to understanding the dynamic behavior of two-phase systems influenced by both thermal and mechanical processes.

How to cite: Frasunkiewicz, J., Kaus, B., Popov, A., Schuler, C., and Riel, N.: Leveraging Differentiable Programming in Julia: Forward and Inversion Modeling of Two-Phase Systems, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10269, https://doi.org/10.5194/egusphere-egu25-10269, 2025.

EGU25-10823 | ECS | Posters on site | GD10.1

Parameter Sensitivity Analysis of Plate Motion using the Adjoint Method and Automatic Differentiation 

Christian Schuler, Albert de Montserrat, Jacob Frasunkiewicz, Pascal Aellig, and Boris Kaus

The adjoint method for the Stokes equations provides a versatile and highly efficient approach to investigate the underlying physics of geodynamic processes. Reuber et al. (2018) demonstrated that adjoint sensitivities can be used to develop scaling laws for processes like folding and subduction dynamics. The gradients derived using the adjoint method can also directly be used in inversions in geodynamic applications. However, previous implementations of the adjoint method have typically been highly problem-dependent and often limited to viscous rheologies. Extending it to other nonlinear rheologies typically required substantial additional work, which is likely one of the reasons that the method has not yet been widely adopted in solid Earth geosciences.

To overcome this problem, we use automatic differentiation (AD) to compute the gradients needed to develop an adjoint solver for the Stokes equations. The gradients are computed using the Julia package Enzyme.jl. The adjoint solver is designed to be problem-agnostic, where the gradients are automatically computed for any user-defined rheology, from a simple linear viscous model to a complex visco-elasto-viscoplastic composite rheology. This functionality is added to the JustRelax.jl thermo-mechanical solver, where we use the same pseudo-transient solver strategy to solve both the forward and adjoint problems. This approach ensures that the adjoint solver remains consistent and fully generic.

The method is applied to analyse horizontal plate motion around subduction zones. For different material parameters, it is possible to calculate sensitivity kernels that show, for each location in the numerical domain, how much these parameters influence the horizontal plate motion (e.g. Reuber et al (2020)). The scaling of sensitivities for different parameters is discussed to enable a quantitative comparison. This approach is then used to identify the most influential factors affecting plate motion.

 

Reuber, G. S., Popov, A. A., & Kaus, B. J. (2018). Deriving scaling laws in geodynamics using adjoint gradients. Tectonophysics, 746, 352-363.

Reuber, G. S., Holbach, L., Popov, A. A., Hanke, M., & Kaus, B. J. (2020). Inferring rheology and geometry of subsurface structures by adjoint-based inversion of principal stress directions. Geophysical Journal International, 223(2), 851-861.

 

How to cite: Schuler, C., de Montserrat, A., Frasunkiewicz, J., Aellig, P., and Kaus, B.: Parameter Sensitivity Analysis of Plate Motion using the Adjoint Method and Automatic Differentiation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10823, https://doi.org/10.5194/egusphere-egu25-10823, 2025.

EGU25-11462 | Posters on site | GD10.1

Physics-based and physics-agnostic reduced order modeling 

Alberto García-González and Sergio Zlotnik

In this work we describe dimensionality reduction methods to solve parametric problems governed by partial differential equations (PDE). The goal of these methodologies is to elucidate and reduce the dimensionality of the manifold containing the family of solutions of a parametric problem. This leads to a reduced system that can often be solved in real time. These techniques are being successfully applied in many fields in science and engineering, e.g. [1,2] as well as in geodynamics [3,4].

The application of these techniques involves two phases: i) creation of a reduced space, often done via a sampling of the parametric space and a singular value decomposition, and ii) use of the reduced space to find a new solution within the family.

Here we want to compare methodologies that, in their second step, include or neglect the physics described by the PDEs. We call these, physics-based and physics-agnostic approaches. Reduced Basis methods being an example of the first, and surrogate modelling one of the second.

Applications of flow in porous media are used as examples to test the strengths and weaknesses of the different approaches. These methodologies are a potential tool to be used in situations where it is unaffordable to obtain a very large training set (big data).

REFERENCES

[1] Rocas M., A. García-González, S. Zlotnik, X. Larráyoz and P. Díez. Nonintrusive Uncertainty Quantification for automotive crash problems with VPS/Pamcrash. Finite Elements in Analysis & Design, Vol. 193, doi:10.1016/j.finel.2021.103556, 2021.

[2] Muixí A., S. Zlotnik, P. Calvet, M. Espanol, I. Lodoso-Torrecilla, M.P. Ginebra, P. Díez and A. García-González. A multiparametric advection-diffusion reduced-order model for molecular transport in scaffolds for osteoinduction. Biomechanics and Modeling in Mechanobiology, doi:10.1007/s10237-022-01577-2, 2022.

[3] Ortega O., S. Zlotnik, J.C. Afonso and P. Díez. Fast Stokes flow simulations for geophysical-geodynamic inverse problems and sensitivity analyses based on reduced order modeling. Journal of Geophysical Research: Solid Earth, Vol. 125, 1–25, doi:10.1029/2019JB018314, 2020.

[4] Manassero M., J.C. Afonso, F. Zyserman, A. Jones, S. Zlotnik and I. Fomin. A Reduced Order Approach for Probabilistic Inversions of 3D Magnetotelluric Data II: Joint inver- sion of MT and Surface-Wave Data. Journal of Geophysical Research - Solid Earth, doi:10.1029/2021JB021962, 2021.

How to cite: García-González, A. and Zlotnik, S.: Physics-based and physics-agnostic reduced order modeling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11462, https://doi.org/10.5194/egusphere-egu25-11462, 2025.

EGU25-11537 | ECS | Posters on site | GD10.1

1D modelling of pegmatite migration 

Mathis Bergogne, Laetitia Le Pourhiet, Ludovic Räss, and Alexis Plunder

Pegmatites and rare metal granites are granitic igneous rocks distinguished by their texture, which is dominated by crystal growth. These rocks are frequently enriched in rare elements (e.g., Li, Cs, Be, Nb, Ta) and represent economically significant deposits, classified among the critical raw materials identified by the European Commission. Our objective is to better constrain the tectonic parameters that govern the emplacement of pegmatites within the continental crust, including their migration rates and durations, with a particular emphasis on the role of temperature in these crustal migration processes.

To model those fluid migrations, two-phase flow in Julia, based on porosity waves with compressible fluid is used. The porosity is interpreted as melt [1]. To improve the yet existing codes [2], we implement temperature in our two phase flow formulation from energy conservation. Temperature allow a thermomechanical coupling with rock viscosity. A first equation with a simple exponential coupling is used to understand thermal implication on viscosities.

The model represents a continental crust with partial melting occurring within the lowermost 5 km, where temperature is maintained at 750°C due to underplating. A constant geothermal gradient is applied from this depth to the surface. A 10% porosity anomaly is introduced in the partially molten zone, while a baseline porosity of 1% is applied throughout the model to ensure numerical stability. The fluid viscosity is set at 10^4 Pa.s, while at 750°C, the rock viscosity is 10^16 Pa.s. A constant permeability of 10^-11 m² is applied throughout the model. Thermomechanical couplings of varying strength are implemented to assess their impact on migration processes. Accordingly, the rock viscosity at 450°C is varied between 10^16Pa.s and 10^21 Pa.s.

Models reveals two distinct mechanisms that halt migration. The first occurs when the thermomechanical coupling is low (soft and hot crust). Allowing rock viscosity to remain low, so melt migration can outpace thermal diffusivity. Enabling the melt to be in an undercooling state. This means that the magma can migrate beyond the point at which the surrounding rock reaches the crystallization temperature of the melt, a necessary condition for pegmatite formation. The second case arises when thermomechanical coupling is strong, causing the surrounding rock's viscosity to become too high for the magma to reach undercooling condition. In this scenario, the magma crystallizes as soon as it reaches the surrounding rock at its crystallization temperature, potentially becoming trapped by a viscous layer (of different or colder nature).

The use of a geothermal gradient more representative of a metamorphic core complex, along with an improved thermomechanical coupling, should refine the estimates of migration time and distance. Similarly, the introduction of viscous heterogeneity would help highlight the geological structures that may or may not facilitate the migration of these magmas to shallower levels of the crust.

 

References:

[1] L. Räss, T. Duretz & Y.Y. Podladchikov (2020). https://doi.org/10.1093/gji/ggz239

[2] A. Plunder & al. (2022). https://doi.org/10.1016/j.lithos.2022.106652

How to cite: Bergogne, M., Le Pourhiet, L., Räss, L., and Plunder, A.: 1D modelling of pegmatite migration, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11537, https://doi.org/10.5194/egusphere-egu25-11537, 2025.

EGU25-11825 | Posters on site | GD10.1

Scalable hybrid multigrid for staggered grid discretizations in geodynamics 

Anton A. Popov, Boris J.P. Kaus, and Iskander Ibragimov

The staggered grid finite difference is a robust discretization method for the high-resolution 3D  geodynamic simulations that involve heterogeneous material parameters. Achieving its scalability on parallel machines inevitably requires the application of multigrid solvers. In particular, a coupled velocity-pressure geometric multigrid preconditioner based on Galerkin coarsening scheme demonstrates very good results. However, this method relies on assembled matrices which have a significant memory imprint and prohibits achieving peak performance due to suboptimal use of the limited memory bandwidth. A geometric multigrid method, based on the re-discretization of linear operators on the coarser levels, converges generally slower, but can be implemented  in a completely matrix-free manner. It poses a valuable alternative to the Galerkin method, since an increased number of iterations can be compensated by a greater performance of the matrix-vector products computed on the fly without storing matrices in the memory.

Here we present a hybrid approach that allows optimal combination between various types of coarsening techniques for staggered grid discretizations. This work is performed within the framework of ChEESE-2p project (Centre of Excellence for Exascale in Solid Earth) and involves the flagship code LaMEM (Lithosphere and Mantle Evolution Model), which is based on Portable Extensible Toolkit for Scientific computation (PETSc), following an approach suggested for finite element discretizations by May et al. (2015). Here, we extend it to the staggered grid finite difference, discuss the optimal solver parameter selection, and document performance gains that can be achieved by using the matrix-free operators.

We typically start with a few levels of re-discretized matrix-free operators, followed by Galerkin geometric coarsening operating on assembled matrices. This approach ensures that most of the optimization and memory saving is already obtained at the top levels, whereas more robust Galerkin coarsening can be used at coarser levels without compromising the convergence. At the coarse grid level, we either utilize a parallel sparse direct solver or a black-box algebraic multigrid method.  The number of processors participating in a coarse grid solve can be optimally selected via PETSc sub-communicator framework (Telescope). 

D. A. May, J. Brown, L. Le Pourhiet, 2015. A scalable matrix-free multigrid preconditioner for finite element discretizations of heterogeneous Stokes flow, Comput. Methods Appl. Mech. Engrg., 290, 496–523.

How to cite: Popov, A. A., Kaus, B. J. P., and Ibragimov, I.: Scalable hybrid multigrid for staggered grid discretizations in geodynamics, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11825, https://doi.org/10.5194/egusphere-egu25-11825, 2025.

I present a set of numerical experiments, which show the formation, evolution, and influence of small-scale rolls at the lithosphere-asthenosphere boundary (LAB). The rolls originate from lateral gradients of temperature and are not related to classical large-scale Rayleigh–Bénard convection. Rather, they represent a form of horizontal convection, arising from the circumstance that the lower part of the lithosphere (both oceanic and continental) can contribute to the advection of material (due to a relatively low viscosity) but is characterized by a non-adiabatic thermal regime. The formation of convection rolls indicates that the process is relatively steady, with a relaxation time of several hundreds kyrs. Although the LAB geometry influences the formation of convective cells, these features form even in presence of a flat LAB surface, whenever there is a lateral thermal change within the lithosphere, for example at the transition between oceanic and continental lithosphere along continental margins. An important observation is that the thermal structure of the oceanic lithosphere close to a spreading center induces an ascending flow even in absence of extension. Consequently, an active component of spreading exists regardless of whether two plates are moving apart. In these experiments, the active component of spreading induces a velocity between 0.6 and 1.2 cm/yr, which adds to the velocity imposed with boundary conditions. Such active component develops even in the case of closed systems and determines a state of compressional stress within the lithosphere. The structure of the ascending flow in the melting regime below a spreading center suggests that it results from the superposition of two small-scale rolls with opposite polarity, associated with horizontal convection.

How to cite: Schettino, A.: The role of small-scale horizontal convection in lithosphere-asthenosphere interaction, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12536, https://doi.org/10.5194/egusphere-egu25-12536, 2025.

EGU25-13428 | Orals | GD10.1

Harnessing Neural Network and Operators to Simulate Subsurface Geomechanical Processes  

Lawrence Hongliang Wang and Viktoriya Yarushina

Simulating subsurface geological processes, such as compaction-driven fluid flow and rock deformation, is essential for understanding natural phenomena and addressing challenges in energy production and resource extraction. Traditional numerical methods, while effective, are computationally expensive and struggle to efficiently model large-scale dynamical problem in subsurface systems. This creates a bottleneck for large-scale simulations and real-time decision-making. Recent advances in machine learning (ML) offer promising solutions to enhance simulation efficiency. Neural operators, which learn mappings between function spaces, provide a flexible, scalable approach to modeling complex systems. Unlike traditional methods, neural operators can generalize across varying inputs and geometries, offering a more efficient and versatile alternative. This study explores the potential of advanced machine learning techniques, specifically Fourier Neural Operators (FNO) and Physics-Informed Neural Operators (PINO), to model two critical subsurface geomechanical processes: compaction-driven fluid flow and elastic stress analysis for tunnelling.

For the first case, numerical simulations were conducted to generate a dataset of up to ~10,000 samples, derived from ~1,000 different initial porosity conditions represented by randomly generated polygons. The FNO model was trained using Nvidia A100 GPUs (80G). Training loss decreased rapidly during early epochs and stabilized below 0.02 after approximately 50,000 epochs. Models trained with larger datasets (e.g., 9,753 samples) demonstrated significantly improved validation performance, achieving a validation loss of ~0.06. In contrast, models trained on smaller datasets exhibited overfitting, with validation losses exceeding 0.3. The trends in validation loss, evaluated using 60 test cases with elliptical initial conditions excluded from the training data, underscored the importance of dataset size in enhancing model generalization for machine learning-based geological simulations. The validation results demonstrated high predictive accuracy, with maximum errors below 10%. Models trained on larger datasets achieved superior performance, particularly for cases with sharper structural features. These findings highlight the capability of FNO models to effectively generalize and reproduce the dynamics of complex fluid flow in subsurface environments. The second case focuses on elastic stress analysis for tunneling, where stresses and deformations around underground excavations are critical to ensuring structural stability. Preliminary efforts have been directed toward generating numerical datasets to train FNO and PINO models, with the goal of capturing stress distribution and deformation patterns under diverse geological and engineering conditions. While results are still emerging, early indications suggest that PINO may provide additional advantages by incorporating physical laws directly into the training process, potentially reducing the amount of data required and improving computational efficiency.

This work demonstrates the transformative potential of neural operators in addressing computational challenges associated with subsurface geomechanical modeling. By combining the flexibility of data-driven methods with the robustness of physics-informed approaches, FNO and PINO offer scalable and efficient alternatives to traditional numerical methods.

How to cite: Wang, L. H. and Yarushina, V.: Harnessing Neural Network and Operators to Simulate Subsurface Geomechanical Processes , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13428, https://doi.org/10.5194/egusphere-egu25-13428, 2025.

EGU25-14096 | ECS | Orals | GD10.1

Extreme-Scale Geodynamic Modelling with TerraNeo 

Ponsuganth Ilangovan, Nils Kohl, Marcus Mohr, Hamish Brown, Eugenio D'Ascoli, Isabel Papanagnou, Berta Vilacis, and Hans-Peter Bunge

Finely resolved Geodynamic mantle convection models are crucial to understand
the detailed physics governing major geological process and to infer
the mineralogical state of the Earth. Given the scale needed to globally
resolve features of the mantle such as unstable boundary layers
and asthenospheric flows where viscosity can change by around four orders of
magnitude within 50 km, traditional sparse matrix methods become unsuitable
due to their immense memory requirements. TerraNeo builds upon the
massively parallel matrix-free finite element framework HyTeG which uses
geometric multigrid solvers on block-structured hybrid tetrahedral grids.
The extreme scalability of HyTeG has been demonstrated previously, solving
Stokes problems with trillions (1e12) of unknowns, corresponding to ≃ 1
km global resolution of Earth’s mantle.
We discuss the features and scalability of TerraNeo with respect to the
numerical treatment of the truncated anelastic liquid approximation as a
model for mantle convection. The compute kernels are evaluated and verified
through geophysical applications, convergence studies, and community
benchmarks covering sharp viscosity variations, nonlinear rheologies and
mixed boundary conditions.

How to cite: Ilangovan, P., Kohl, N., Mohr, M., Brown, H., D'Ascoli, E., Papanagnou, I., Vilacis, B., and Bunge, H.-P.: Extreme-Scale Geodynamic Modelling with TerraNeo, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14096, https://doi.org/10.5194/egusphere-egu25-14096, 2025.

EGU25-15996 | Orals | GD10.1

Adaptive FEM-DEM bridging coupling to study third-body/gouge evolution 

Guillaume Anciaux, Manon Voisin-Leprince, and Jean-François Molinari

The behavior of interfaces in seismic faults, and tribological systems in general, is governed by the interaction of discrete microconstituents trapped between contacting surfaces, often referred to as the gouge or the third-body. This is an amorphous wear particle agglomeration undergoing significant deformation, while the surrounding regions experience comparatively moderate strain. Understanding the dynamics of such systems, and in particular the evolution of the third body, can rely on particle-based numerical models such as the Discrete Element Method (DEM). The predicted behavior of the gouge can be sensitive to the boundary conditions, and therefore to the system size. However, the important computational costs prevent handling arbitrarily large domain sizes, which calls for cheaper Discrete-Continuum coupled methods. To accurately capture the behavior of continuum (long-range boundary) and discrete regions (gouge), we employed a hybrid modeling strategy combining the Finite Element Method (FEM) for continuum regions and the Discrete Element Method (DEM) [1,2].

To accommodate the evolving nature of the third body and prevent limitations imposed by the size of the discrete region, we will introduce in this presentation an adaptive coupling. This approach allows FEM regions to transition dynamically into DEM regions when a sufficient deformation criterion is met. Such a condition is evaluated within the third body near the coupling region. The adaptive framework supports large-scale simulations, and it will be demonstrated to support amorphous and ordered (crystalline) material setups for a gouge. Finally, the adaptive coupling is used to model the evolution of a third body comprising elliptical rigid bodies, which will be shown to impact the gouge evolution in certain conditions. Our findings underscore the importance of coupling techniques in modeling the complex, multiscale nature of frictional interfaces and contribute to a deeper understanding of the role of granularity in dynamic friction and third-body evolution.

[1] Xiao, S. P. and T. Belytschko (2004). “A bridging domain method for coupling continua with molecular dynamics”. Computer Methods in Applied Mechanics and Engineering. doi: 10.1016/j.cma.2003.12.053
[2] Voisin-Leprince, M., J. Garcia-Suarez, G. Anciaux, and J.-F. Molinari (2022). “Finite element method–discrete element method bridging coupling for the modeling of gouge”. International Journal for Numerical Methods in Engineering. doi: 10.1002/nme.7171

How to cite: Anciaux, G., Voisin-Leprince, M., and Molinari, J.-F.: Adaptive FEM-DEM bridging coupling to study third-body/gouge evolution, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15996, https://doi.org/10.5194/egusphere-egu25-15996, 2025.

EGU25-16111 | ECS | Posters on site | GD10.1

Variational Stokes: free surface for staggered grid finite differences schemes for geodynamic and ice flow modelling 

Albert de Montserrat Navarro, Pascal Aellig, Timothy Gray, Ludovic Räss, and Ivan Utkin

In geodynamic models, the incorporation of a free surface boundary condition is crucial to better understand and resolve, for example, the coupled interaction between the lithosphere, deep mantle, and surface processes. A free surface is similarly important in ice flow models to capture the geometry of the ice sheet and its temporal evolution.

While the implementation of a free surface is relatively straightforward in finite element methods due to their capacity to manage complex and deformable geometries, and boundary conditions, the treatment of a free surface boundary (or any other boundary) that is not aligned with the staggered grid of a finite difference (FD) scheme poses a significant challenge. A common approach adopted by FD geodynamic codes, such as I2/3VIS (Gerya and Yuen, 2007) or LAMEM (Popov and Kaus, 2016), involves the incorporation of an additional rheology layer above the surface, simulating the presence of air. However, the of Stokes solvers is constrained by the viscosity contrast occurring within the domain, typically in the range of 6 to 7 orders of magnitude. Consequently, the viscosity of the air layer is limited to values within the 1e16-1e18 Pa*s range. This approach is not only physically unrealistic, but also leads to an inaccurate topography evolution, and introduces a very strong and sharp viscosity contrast at the rock and air interface, which hinders the convergence of iterative solvers particularly the Accelerated Pseudo-Transient (APT) method employed in this study.

To address these limitations, we propose the implementation of a variational Stokes approach (Larionov et al. 2017), which allows for the incorporation of both real free surface and solid wall boundary conditions. This approach is then combined with either a marker chain or a level set to track evolution of the surface. We demonstrate that this approach greatly improves the convergence rate of the iterative APT solver, as well as demonstrate its accuracy and applicability to geodynamic and ice flow simulations with a set of benchmarks and toy codes.

 

Gerya, Taras V., and David A. Yuen. "Robust characteristics method for modelling multiphase visco-elasto-plastic thermo-mechanical problems." Physics of the Earth and Planetary Interiors 163.1-4 (2007): 83-105.

Popov, Anton, and Boris Kaus. "3D modelling of non-linear visco-elasto-plastic crustal and lithospheric processes using LaMEM." EGU General Assembly Conference Abstracts. 2016.

Larionov, Egor, Christopher Batty, and Robert Bridson. "Variational stokes: A unified pressure-viscosity solver for accurate viscous liquids." ACM Transactions on Graphics (TOG) 36.4 (2017): 1-11.

How to cite: de Montserrat Navarro, A., Aellig, P., Gray, T., Räss, L., and Utkin, I.: Variational Stokes: free surface for staggered grid finite differences schemes for geodynamic and ice flow modelling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16111, https://doi.org/10.5194/egusphere-egu25-16111, 2025.

EGU25-16478 | Orals | GD10.1

ASPECT 3.0: The Advanced Solver for Planetary Evolution, Convection, and Tectonics 

Rene Gassmöller, Timo Heister, Wolfgang Bangerth, Juliane Dannberg, Menno Fraters, Anne Glerum, Robert Myhill, and John Naliboff

Modern geodynamic models have become increasingly complex, coupling detailed numerical approximations to many physical processes with large observational datasets. This coupling creates unique challenges for modern research software such as how to combine complex rheologies utilizing multiple flow mechanisms with the simultaneous modeling of mineral microstructure; how to model realistic geometries and evolving surface topography while simultaneously including large observational datasets of topography and surface deformation; and how to utilize highly-optimized and scalable numerical solvers while keeping up with changing high-performance computing architectures.

We here present our approach to reconciling these challenges: The next major release of ASPECT - The Advanced Solver for Planetary Evolution, Convection, and Tectonics. During the six years since our last major release, we have implemented many new features and improvements. Here we report on a new major release that highlights ASPECT's increased flexibility in modeling complex tectonic and convection problems. New features we will present at the workshop are in particular:

  • A new default Stokes solver utilizing a matrix-free geometric multigrid preconditioner
  • Complex rheologies like visco-elasto-plasticity including Peierls-, dislocation-, and diffusion-creep
  • Models of pinned grain-size evolution in a two-mineral assemblage
  • Evolution of crystal-preferred orientation using DREX like algorithms
  • Utilizing modern external libraries for the accurate solution of ordinary differential equations
  • Extended support for efficiently including large-scale datasets in parallel models
  • Interfaces to surface evolution modeling software like Fastscape and others
  • Optimizing finite element type, degree, and advection method for different compositions
  • Major improvements to the structure of the code base, plugin systems, and user interface

As usual the release is open-source and freely available at https://aspect.geodynamics.org/. We hope that providing well-documented, flexible, and tested geodynamic research software provides the community with the necessary tools to tackle the geodynamic research questions of the next decade.

How to cite: Gassmöller, R., Heister, T., Bangerth, W., Dannberg, J., Fraters, M., Glerum, A., Myhill, R., and Naliboff, J.: ASPECT 3.0: The Advanced Solver for Planetary Evolution, Convection, and Tectonics, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16478, https://doi.org/10.5194/egusphere-egu25-16478, 2025.

EGU25-16577 | Posters on site | GD10.1

Differentiable multi-physics solvers for extreme-scale geophysics simulations on GPUs 

Ludovic Räss, Ivan Utkin, Albert De Montserrat, Boris Kaus, Paul Tackley, William Moses, and Thibault Duretz

Although geodynamics and ice flow dynamics address distinct physical systems, they share significant computational and modelling challenges. Both require vast, data-intensive simulations on next-generation high-performance computing (HPC) platforms. With limited observational data, these models must be rigorously constrained to improve their predictive power. Our work focuses on differentiable modelling of Earth’s largest ice sheets and high-resolution 3D geodynamic processes, such as magmatic systems and the formation of the Alps.

We are developing differentiable multi-physics solvers for extreme-scale geophysical simulations on GPUs - ∂GPU4GEO. These high-performance, scalable tools leverage advanced programming techniques, particularly automatic differentiation (AD) within the Julia programming language. Using Enzyme.jl, an AD tool integrated with the LLVM compiler, we combine differentiation with compiler optimisations. This approach enables highly efficient reverse-mode AD, achieving near-theoretical peak performance.

Building on the GPU4GEO PASC project (2020–2024), we are extending pseudo-transient solvers with differentiable modelling capabilities. The modular GPU4GEO software stack, composed of specialised Julia packages, provides solvers for diverse physical systems and customisable building blocks. By integrating Enzyme.jl into the entire stack, we enable high-performance AD on GPUs while maintaining support for distributed-memory parallelism via MPI. These developments ensure scalability on flagship supercomputers and facilitate efficient exploration of geophysical processes.

This collaborative effort targets applications requiring large-scale simulations to address critical scientific challenges. The resulting computational tools are optimised for next-generation GPU architectures, offering transformative potential for geodynamics and glaciology research.

How to cite: Räss, L., Utkin, I., De Montserrat, A., Kaus, B., Tackley, P., Moses, W., and Duretz, T.: Differentiable multi-physics solvers for extreme-scale geophysics simulations on GPUs, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16577, https://doi.org/10.5194/egusphere-egu25-16577, 2025.

EGU25-17228 | ECS | Orals | GD10.1

On the Application of Compatible Finite Elements for Divergence-Free and Mesh-Independent Viscoelastic-Plastic Rheology in Geodynamics Simulations 

Karim Norouzi-Moghanjoghi, Javier García-Pintado, and Marta Perez-Gussinye

The movement of the Earth's crust and mantle in geodynamics is typically modeled as the flow of a viscous fluid governed by the Stokes equations. Incorporating plasticity into material rheology often results in mesh-dependent behavior, which poses challenges for accurate numerical simulations. Several approaches have been proposed to mitigate mesh dependence and develop solvers that decouple solution errors from viscosity and mesh size.

Traditionally, Taylor-Hood (TH) and Crouzeix-Raviart (CR) elements of order 2 are used for geodynamics simulations. In this study, we examine the numerical solution of variable-viscosity Stokes flow with plasticity and Drucker-Prager type yielding using Scott-Vogelius (SV) compatible finite elements in combination with pseudo-Jacobian and augmented Lagrange methods. The Scott-Vogelius element is unique among finite elements for the mixed formulation of Stokes flow, as it has an associated De Rham complex. This theoretically ensures a divergence-free velocity field. We investigate the degree of decoupling between velocity errors, pressure errors, and viscosity-induced errors in a viscoelasto-plastic case study.

Our results show that Taylor-Hood elements (CG2 × CG1 for velocity and pressure) fail to provide accurate solutions in such cases. While the low-order CR elements perform better, the higher-order SV elements (CG4 × DG3) yield the best results. 

We conclude that due to the inherent mesh-dependent behavior and viscosity dependent errors in TH elements, CR or SV elements should be preferred for geodynamics simulations. 

How to cite: Norouzi-Moghanjoghi, K., García-Pintado, J., and Perez-Gussinye, M.: On the Application of Compatible Finite Elements for Divergence-Free and Mesh-Independent Viscoelastic-Plastic Rheology in Geodynamics Simulations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17228, https://doi.org/10.5194/egusphere-egu25-17228, 2025.

EGU25-17495 | Posters on site | GD10.1

Reconstructing landscapes: an adjoint model of the stream power and diffusion equation. 

Carole Petit, Anthony Jourdon, and Nicolas Coltice

Reconstructing the evolution of a landscape provides insights into its geological and/or climatic history and into processes shaping the earth's surface: what was the configuration of the drainage network before a specific geological or climatic event, what are the areas that are currently most sensitive to fluvial incision or hillslope processes, or to which extent lithological contrasts influenced landscape evolution are frequent questions. Most of the time, these questions are addressed with forward models in which only a small part of the parameter space is explored.

Landscape evolution can be simulated using a diffusion-advection equation where the diffusive term represents hillslope erosion-deposition processes and advection simulates river incision. In this case, the advection velocity can be calculated from drainage area and erodibility parameters of the Stream Power Law.  The model can also include a source term, which simulates tectonic uplift. This approach permits to solve a PDE and formulate an adjoint model that can be used for parameter inversion and sensitivity analysis. In this study, we use the Firedrake package which includes automatic differentiation procedures for building the adjoint model. Our results illustrate different model sensitivities to diffusion and erodibility coefficients, and show that it is able to reconstruct spatial variations of these coefficients.

We then apply the adjoint model to sensitivity analysis and to parameter inversion in real-world cases. The first one is the southeastern border of the French Massif Central, for which we seek at understanding what was the topography prior to a major incision by tributaries of the Rhone River. The second case is the footwall topography along a segment of the Wasatch normal fault, USA, for which we aim at quantifying temporal uplift rate variations.

In the French Massif Central, inversion of the initial conditions reveals that the pre-incision topography consists of a relatively smooth and flat footwall delimited by a well-defined and linear fault escarpment that corresponds to a Mesozoic normal fault system. In the Wasatch range, the model indicates a significant increase in the uplift rate of the Wasatch Range, from 0.2 to 1 mm.yr-1, since approximately 2 Ma, aligning well with recently published estimates.

How to cite: Petit, C., Jourdon, A., and Coltice, N.: Reconstructing landscapes: an adjoint model of the stream power and diffusion equation., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17495, https://doi.org/10.5194/egusphere-egu25-17495, 2025.

EGU25-17922 | ECS | Posters on site | GD10.1

Retrieving climate proxies from an invertible glacier evolution model. 

Kejdi Lleshi, Guillau Jouvet, and Frédéric Herman

Glacier evolution models (GEMs) are important tools in glaciology to predict future glacier response from climate forcing. However, reconstructing past climates requires inversion tools to infer the climate forcing that explains paleoglacier extents documented through historical records or geomorphic features. 
Such "inverted" GEMs are less common compared to forward GEMs but are important to better constrain climate from the past. 
For instance, Visnjevic et. al proposed a model to estimate the Equilibrium Line Altitude (ELA) from reconstructed paleoglacier extents. 
However, their approach assumes stationary glaciers, neglecting temporal dynamics, and employs a heuristic inversion technique.

Recent implementations of automatic differentiation (AD), coupled with Graphic Processing Unit (GPU) performance improvements, provide a promising pathway to develop fully differentiable and computationally efficient GEMs. Here, we introduce an Invertible Glacier Evolution Model (IGEM), a new framework designed to overcome the limitations of existing inversion methods.
Our IGEM relies on the Shallow Ice Approximation (SIA)  for the ice flow, and surface mass balance is computed with the Positive Degree Day (PDD) .
The model’s tensor-based architecture leverages GPU acceleration and enables efficient computation of gradients with respect to input climate variables, such as temperature and precipitation, which are used for PDD calculations. The gradient-descent inversion scheme employed in our IGEM converges more rapidly, delivers more accurate solutions, and offers greater generality (e.g., it is not constrained by the stationary assumption) compared to heuristic inversion methods.

The main challenge here is due to the fact that one forward GEM simulation requires thousands of iterations to model a glaciation spell.
To compute the gradient of the cost function with respect to climate forcing, a chain derivation of all operations within the forward GEM is necessary, which is memory-challenging, especially on GPUs.
To address this, our IGEM selectively recomputes a subset of intermediate operations during gradient computation. Instead of storing all operations, only those essential for computing gradients are cached, while others are recomputed during the "backward" pass. This approach reduces memory usage at the cost of increased computation time, enabling the methodology to handle large-scale problems effectively.

To illustrate the feasibility of our approach, we apply it to the inference of climate proxies at the Aletsch Glacier for the period 1880–2010. We leverage sequentially dated observations of the glacier geometry during the same timeframe. Given the nonuniqueness of the problem, the method permits the derivation of a set of compatible temperature and precipitation proxies, which are evaluated against weather station data near the glacier.

This proof-of-concept shows that our IGEM approach enables the extraction of compatible climate proxies, such as temperature and precipitation, provided documented glacier former extents. By bridging the gap between glacier dynamics and climate reconstruction, our IGEM has the potential to advance our understanding of past climates in formerly glaciated regions.

How to cite: Lleshi, K., Jouvet, G., and Herman, F.: Retrieving climate proxies from an invertible glacier evolution model., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17922, https://doi.org/10.5194/egusphere-egu25-17922, 2025.

EGU25-19536 | Posters on site | GD10.1

Automatic tuning of iterative pseudo-transient solvers for geodynamic modelling 

Thibault Duretz, Albert de Montserrat, Rubén Sevilla, Ludovic Räss, and Ivan Utkin

Geodynamic modeling has become a crucial tool for investigating the dynamics of Earth deformation across various scales. This approach involves solving mechanical problems characterized by significant property variations (e.g., viscosity, shear modulus, conductivity) under nearly incompressible conditions. Recent advancements in technology have facilitated the development of iterative pseudo-transient solvers, which require minimal global communication and enable near-optimal parallel scaling on supercomputers. However, selecting numerical parameters that ensure both robust and rapid convergence remains a challenging task. In this contribution, we explore potential strategies to address these challenges and provide application examples using both finite difference and face-centered finite volume methods.

How to cite: Duretz, T., de Montserrat, A., Sevilla, R., Räss, L., and Utkin, I.: Automatic tuning of iterative pseudo-transient solvers for geodynamic modelling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19536, https://doi.org/10.5194/egusphere-egu25-19536, 2025.

EGU25-20446 | ECS | Posters on site | GD10.1

Probing Earth’s interior with neutrinos: sensitivity kernels for a 1-dimensional Earth model 

Isabel Astrid Goos, João A. B. Coelho, Yael A. Deniz Hernandez, Stephanie Durand, Nobuaki Fuji, Eric L. Mittelstaedt, Rebekah Pestes, and Véronique Van Elewyck

Neutrino oscillation tomography is potentially a method for probing the properties of Earth's deep interior, complementing classical geophysical and geochemical methods. It relies on the detection of neutrinos, subatomic particles that interact weakly with matter and can traverse the Earth’s interior essentially unimpeded. Neutrinos exist in three types, called "flavors": electron, muon, and tau. As they propagate, they can change from one flavor to another, a phenomenon known as neutrino oscillation. Oscillation probabilities are influenced by the electron density profile along the neutrino’s path, determined by the matter density and the proton-to-nucleon ratio (Z/A) distribution. By measuring neutrino oscillations, it is thus possible to retrieve information about the composition and density variations in the Earth’s interior. 

In this work, we present sensitivity kernels from neutrino oscillation tomography for a spherically symmetric Earth model. Our goal is to identify which depth ranges can be effectively studied using this technique. To understand the constraints that neutrino oscillation tomography can provide on Earth's structure, we first model the sensitivity of neutrino tomography to the planet's composition and density assuming an ideal neutrino detector. Then, to derive realistic sensitivities, we apply the detector’s response (i.e., resolution) of next-generation neutrino telescopes. We show that an ideal detector is most sensitive to the outer core, while realistic detectors with lower resolution but large detection volumes shift the sensitivity focus to shallower depths. Finally, we discuss how this method could provide complementary insights into the structure of large low velocity provinces (LLVPs) at the base of mantle and the water content in the mantle transition zone (MTZ).

How to cite: Goos, I. A., Coelho, J. A. B., Deniz Hernandez, Y. A., Durand, S., Fuji, N., Mittelstaedt, E. L., Pestes, R., and Van Elewyck, V.: Probing Earth’s interior with neutrinos: sensitivity kernels for a 1-dimensional Earth model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20446, https://doi.org/10.5194/egusphere-egu25-20446, 2025.

EGU25-20801 | Posters on site | GD10.1

The Thermal Lattice Boltzmann Method: new developments, strong scaling to 300K cores, and potential to yield major advancements in geodynamics 

Peter Mora, Gabriele Morra, Craig O'Neill, Leila Honarbakhsh, Jian Kuang, and Amen Barges

The Thermal Lattice Boltzmann Method (TLBM) offers an alternative to classical PDE based solvers for planetary dynamics and is based on solving the Boltzmann Equation on a discrete lattice which maps perfectly onto parallel computers. We present strong scaling performance runs on the Shaheen III HPC cluster at KAUST using up to 300K cores for a 3D whole mantle model at a 3km grid resolution. Based on the throughput performance achieved, the TLBM can model mantle simulation in 3D for one convection cycle's worth of physical time in less than a day of CPU at a 3km resolution. We present 2D performance results which indicate that the TLBM can model ultra-high Rayleigh numbers in 2D well into the ultimate turbulent regime up to Ra = 1018 on 300K cores in a 1x1 aspect ratio model. We also  present an update of the status of TLBM developments and example runs and run times of: (1) the transition to plate tectonics in the Archean using a temperature dependent viscosity, a yield stress formulation of the rheology and partial melting, (2) high Rayleigh number simulations in the turbulent regime up to Ra = 1015 in 2D, (3) 2D whole mantle modelling in a circular annulus and accuracy benchmarks against ASPECT, and (4)  3D simulations of whole mantle convection at a resolution of 30 km on just 96 cores, and (5) iron droplets from an impactor on a turbulent magma ocean settling to form the iron core using a combined TLBM and multiphase LBM. We believe that the TLBM and multiphase TLBM have the potential to lead to new insights in the dynamics and evolution of the Earth and exoplanets from the early lava world stage onwards including plate tectonics due to their high throughput performance and near linear scaling to 100s of K cores. These capabilities enable geodynamical modelling with never-before-seen resolutions in 2D and 3D, high Rayleigh numbers well into the ultimate turbulent regime, studies of turbulent magma oceans and core formation, and phase space studies of planetary dynamics.

How to cite: Mora, P., Morra, G., O'Neill, C., Honarbakhsh, L., Kuang, J., and Barges, A.: The Thermal Lattice Boltzmann Method: new developments, strong scaling to 300K cores, and potential to yield major advancements in geodynamics, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20801, https://doi.org/10.5194/egusphere-egu25-20801, 2025.

GI6 – Multidisciplinary approaches on geoscience instrumentation technologies and systems

EGU25-698 | ECS | Posters on site | GI6.2

Modeling Land Surface Temperature Using UAV-Derived RGB and NIR Data Through Machine Learning Techniques 

Oleksandr Hordiienko and Jakub Langhammer

Land Surface Temperature (LST) estimation is an important part of climate research, helping understand surface heat and environmental changes. This study introduces a simple and innovative way to estimate LST using machine learning and data collected by unmanned aerial vehicle (UAV). The UAV used RGB and near-infrared (NIR) sensors, which are commonly available and affordable.

The research took place in the Šumava Mountains of the Czech Republic, an area with unique landscapes and sensitive ecosystems. The UAV surveys used two types of cameras: one combined RGB and NIR sensors to capture visual and near-infrared data, and the other was a thermal camera to measure ground temperature. The thermal images provided the training data for machine learning models, which were designed to estimate LST using only RGB and NIR data. To test and validate the model, an integrated approach is used: sensors installed in different land cover types, direct measurements of air temperature from ground stations and medium-resolution satellites with a thermal band. This correlation with reference temperature sources ensures the model reflects real thermal conditions rather than relative differences alone. This method can be very useful when thermal cameras are not available, as they are often expensive and need careful calibration.

The models created in this study showed good accuracy, with strong agreement between the predicted and actual LST values but it is still necessary to check the LST directly. Incorporating reference temperature values enhances the model’s accuracy and applicability, allowing for consistent results. This means the models can reliably predict LST using just RGB and NIR data. This approach offers a practical alternative to traditional thermal measurements, which are more costly and harder to use for large-scale or frequent studies. One key advantage of this method is its affordability and ease of use. RGB and NIR sensors are much more accessible than thermal cameras, making it possible for researchers with limited budgets to monitor LST  effectively. 

This study offers a novel method for estimating LST by combining UAV technology, RGB and NIR sensors, and machine learning. The results show that the proposed approach is reliable and applicable for environmental and climate research. By integrating reference temperature sources, this study overcomes the challenges of relative-only measurements, providing reliable LST values for diverse applications. By overcoming the challenges of direct thermal measurements, this method provides an easier way to monitor land surface temperatures across different environments.

How to cite: Hordiienko, O. and Langhammer, J.: Modeling Land Surface Temperature Using UAV-Derived RGB and NIR Data Through Machine Learning Techniques, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-698, https://doi.org/10.5194/egusphere-egu25-698, 2025.

 Elevated flare is the utter most significant exhaust source in chemical plants and as well as the best way to centralized disposal of combustible gases at high altitude. It is considerable to monitor the concentration of the exhaust plume of flares, however, flare research over the past decade has increasingly illustrated that there is likely no one effective method can accomplish the task. Passive Fourier Transform Infrared Spectroscopy (FTIR) remote sensing system is widely used in the field of hazardous chemicals park monitoring and warning, gas distribution monitoring at the scene of the explosion in the way of non-contact long-distance remote sensing. Compared to active FTIR absorption spectrometry, it is easier to install because the hot gas just has to be in the field of view of the telescope of the spectrometer and once there is equivalent radiation bright temperature difference between the measured plume and the background, IR radiation emitted by exhausts or gas plumes is detected and remote sensing by passive FTIR spectrometry allows the retrieval of column densities or concentrations of molecules in gas plumes such as exhaust plumes of aircraft, smoke stacks and flares. In the paper, the exhaust plumes of two elevated flare in a chemical plant in Shanghai is measured by passive FTIR remote sensing system and quantitative the concentrations of CO, N2O, HCN, NH3, C3H3N, C3H6 and C2H4 in the plumes. The theory and process relate with radiometric calibration and calculation of transmittance is presented as well as the factors caused the error of the concentrations of target gases is analysed. The passive FTIR remote sensing system makes up the inability of measure the exhaust plume of flares and provide the efficient and powerful date for estimate/evaluate the combustion process and efficiency of flare, building the list of emission index and so on

How to cite: Han, X. and Li, X.: Remote Sensing for Flaming Plume of Elevated Flares with Passive Fourier Transform Infrared Spectroscopy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2387, https://doi.org/10.5194/egusphere-egu25-2387, 2025.

EGU25-2557 | ECS | Posters on site | GI6.2

Assessing contemporary global land cover products to study land cover change in Poland 

Mahsa Shahbandeh Vayghan, Dominik Kaim, and Jacek Kozak

The availability of global land cover products has been increasing recently, however, its regional quality differs substantially. In this work, the contemporary global datasets including Google’s Dynamic World (GDW), ESA’s World Cover (ESA WC), Esri Land Cover (ELC) map were compared in Poland to assess their usefulness for the forest cover change studies in Central-European conditions. We grouped land cover categories of the three global datasets into 6 land cover classes (forest, semi-natural vegetation, cropland, built-up area, water and other). To assess the accuracy of the global products we used the EU Land Use/Cover Area Frame Survey (LUCAS) points. The results showed that precision for forest class was higher for ESA WC (0.92) than for the other two products (ELC: 0.85; GDW 0.41). Forest class accuracy was the highest for ELC (0.92) and lower for ESA WC (0.90) and GDW (0.81). Overall, ELC had the highest F1 score for the forest class (0.76), slightly higher than ESA WC (0.71), with GDW showing a significantly lower value of 0.57. Our analysis indicated that for forested areas ELC performed better than two other global products, suggesting its usefulness for forest cover change studies in Central Europe.

Acknowledgements:

This research was funded in whole or in part by the National Science Centre, Poland (UMO-2024/53/N/ST10/02518). For the purpose of Open Access, the author has applied a CC-BY public copyright license to any Author Accepted Manuscript (AAM) version arising from this submission.

How to cite: Shahbandeh Vayghan, M., Kaim, D., and Kozak, J.: Assessing contemporary global land cover products to study land cover change in Poland, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2557, https://doi.org/10.5194/egusphere-egu25-2557, 2025.

The inland rivers under the geographical pattern of the mountain-basin system in the arid areas of China have special ecosystem types and landscape appearances. The inland river basin, represented by the Tarim River, has given birth to different ecosystem types and landscape appearances of river corridors-vegetation or farmland patches-desert matrix patterns. Through multi-source remote sensing(RS) data, geographic element monitoring data, ecological environment statistical survey data, model simulation and other multi-source data, the data verification and normalization are carried out, and the ecological environment quality(EEQ) characteristics are obtained through model operation and analysis.The results show that due to the constraints and influences of the mountain-basin system, precipitation shortage, strong evaporation, and severe drought lead to the widespread salinization of the basin. In addition, the sparse vegetation and the frequent occurrence of sandstorm disasters have led to drastic changes in the spatiotemporal dynamics of desertification. Under the multiple stresses of climate change and the development of man-made water resources and land resources, a series of changes have taken place in the EEQ. The analysis of panchromatic aerial RS images (1959), color aerial RS images (1992), JERS-1 OPS RS images (1995) and MODIS RS images (2023) shows that desert riparian forests show a discontinuous distribution on the north and south sides of the main stream corridor, and the vegetation tends to be degraded from the source area to the upper, middle and lower reaches of the main stream. Since 2000, the water resources allocation project in the basin has alleviated the vulnerability of water resources to spatiotemporal changes, slowed down the degradation trend of EEQ in the basin, and significantly improved the EEQ in some areas.Based on the systematic analysis of multi-source data such as hydrology, soil, climate, vegetation and landscape pattern changes in the basin, combined with the SSP climate scenario model, it is found that the future temperature and precipitation will show an upward trend under the SSP2-4.5 and SSP5-8.5 scenarios. Through the establishment of the ecological risk index (ERI) model, the quantitative evaluation showed that the ERI values of the Aksu River Basin in the headwaters were 0.08 and 0.06 in 1998 and 2023, respectively, indicating that the EEQ was in a stable and improving state in the past 25 years, and the EEQ continued to improve. It is estimated that by 2040, drought and flood disasters in the basin will be further aggravated, and the evolution of EEQ will be complex and uncertain.

How to cite: Ranghui, W.: Evolution of ecological environment quality in China's inland river basin based on multi-source data and model analysis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4052, https://doi.org/10.5194/egusphere-egu25-4052, 2025.

EGU25-5453 | ECS | Posters on site | GI6.2

Evaluation of the Impact of NO2 in Atmospheric Correction for Surface Reflectance Estimation 

Seungwon Kim and Kyung-soo Han

The global increase in fine particulate matter, particularly in East Asia, has emphasized the importance of satellite-based monitoring for rapid and extensive observation of atmospheric changes. In South Korea, the Geostationary Environment Monitoring Spectrometer(GEMS) has been deployed to monitor air quality, including aerosol optical depth(AOD). The accuracy of AOD retieval relies significantly on surface reflectance, which is typically estimated using the minimum reflectivity method. However, this approach has limitations as it does not only account for observation geometry conditions(such as SZA, VZA) but also atmospheric conditions such as nitrogen dioxide(NO2) concentrations, which can significantly influence surface reflectance calculations.

This study aimed to assess the impact of NO2 concentrations in atmospheric correction for retrieving surface reflectance. By utilizing VLIDORT RTM(Vector Linearized Radiative Transfer Model for the Solution of Inverse Problems), surface reflectance values adjusted for NO2 were evaluated against those calculated without NO2 consideration. The results demonstrate that accounting for NO2 can lead to enhancining the accuracy of surface reflectance retirevals.

The findings of this research suggest the possibility of improving atmospheric correction by considering NO2 as a factor, in surface reflectance estimation for improved products such as AOD retrieval, ultimately leading to accurate fine particulate matter monitoring. These advancements are expected to contribute to various applied research fields, enhancing the utility of satellite-based environmental monitoring systems like GEMS.

Acknowledgement

This research was supported by Particulate Matter Management Specialized Graduate Program through thet Korea Environmental Industry & Technology Institude(KEITI) funded by the Ministry of Environment(MOE).

How to cite: Kim, S. and Han, K.: Evaluation of the Impact of NO2 in Atmospheric Correction for Surface Reflectance Estimation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5453, https://doi.org/10.5194/egusphere-egu25-5453, 2025.

EGU25-5752 | ECS | Orals | GI6.2

Stromboli Fires: What could have happened? 

Roberto Guardo, Giuseppe Bilotta, Gaetana Ganci, Francesco Zuccarello, Daniele Andronico, and Annalisa Cappello

Between 2019 and 2022, multiple fires affected Stromboli Island, causing significant environmental damage and highlighting the need for effective preventive measures. In 2019, two fires were ignited by eruptive activity, while in 2022, human actions were responsible for a major wildfire. These events underline the complexity of fire dynamics in volcanic environments, where topography, wind, and vegetation flammability play critical roles in fire propagation. Furthermore, the aftermath of these fires has triggered secondary hazards, such as floods and debris flows following heavy rains, which further exacerbated the environmental and societal impact on the island.
In this work we leverage a cellular automata-based numerical model specifically designed for volcanic-induced fires, integrating factors such as wind, topography, and vegetation characteristics to simulate the fire evolution as well as the interaction with possible mitigations measurements. We conducted fire spreading numerical simulations exploring different configurations of firebreak lines, including the strategic use of hiking trails as potential barriers to fire spread. This model also benefits from the integration of Geographic Information Systems (GIS), enhancing its ability to classify soil types and map burnt areas with good spatial accuracy.
The simulations demonstrate how the proposed model can be used to create fire hazard scenarios and evaluate the effectiveness of various mitigation strategies. For instance, our results for the 2019 and 2022 fires exhibit high spatial accuracy, with Brier scores of 0.188±0.002 and 0.073±0.001, respectively. These findings underscore the utility of numerical modeling not only for understanding fire dynamics but also for planning preventive actions to mitigate wildfire risks and reduce the cascading effects of secondary hazards, ultimately contributing to more effective fire and disaster management on Stromboli and other volcanoes with similar environmental conditions.

How to cite: Guardo, R., Bilotta, G., Ganci, G., Zuccarello, F., Andronico, D., and Cappello, A.: Stromboli Fires: What could have happened?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5752, https://doi.org/10.5194/egusphere-egu25-5752, 2025.

Accurate surface reflectance retrieval is crucial for satellite-based Earth observation and various environmental applications. The radiative transfer model (RTM) known as the Second Simulation of a Satellite Signal in the Solar Spectrum vector (6SV) is widely utilized for atmospheric correction of optical satellite data, effectively accounting for various aerosol types and concentrations to derive surface reflectance. However, the accuracy of surface reflectance is significantly affected by the types and concentrations of aerosols in the atmosphere. In particular, anthropogenic aerosols generated from industrialization in East Asia, such as fine particulate matter (PM), constitute a significant proportion of continentally derived aerosols. In this complex atmospheric environment, coastal regions experience a mixture of marine-origin and continent-origin aerosols, which complicates the accurate retrieval of surface reflectance.

Although previous studies have applied 6SV to high-resolution satellite data, comparative analyses of various aerosol types and studies reflecting the characteristics of coastal regions in East Asia remain limited. Therefore, this study focuses on the coastal regions of East Asia, comparing surface reflectance retrieved using standard aerosol models (Continental, Maritime, Urban) provided by 6SV with those officially provided by Sentinel-2A. Additionally, comparisons with surface reflectance derived from aerosol data provided by the AErosol RObotic NETwork (AERONET) were conducted to evaluate the accuracy of each method.

This study is expected to contribute to enhancing the applicability and reliability of remote sensing data by incorporating and analyzing the aerosol characteristics of coastal regions in East Asia.

Acknowledgments

This research was supported by Particulate Matter Management Specialized Graduate Program through the Korea Environmental Industry & Technology Institute(KEITI) funded by the Ministry of Environment(MOE).

 

How to cite: Lee, S. and Han, K.: Comparative analysis of the accuracy of surface reflectance in East Asian coastal areas according to aerosol models based on 6sv rtm, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5754, https://doi.org/10.5194/egusphere-egu25-5754, 2025.

EGU25-7570 | ECS | Orals | GI6.2

Evaluation of different types of satellite images for the identification of minerals formed by Acid Mine Drainage using Spectral Angle Mapping (SAM) 

Joseph Tadeo Almazan Valencia, Denisse Archundia Peralta, and Nelly Lucero Ramírez Serrato

Acid mine drainage (AMD) is a severe environmental issue associated with the generation of finely milled rock waste containing high concentrations of sulfide minerals and potentially toxic elements (PTEs) during mining activities. The formation of secondary minerals, such as sulfates and iron oxyhydroxides, results from sulfide oxidation and subsequent acid neutralization by carbonate and silicate minerals, making them key indicators of AMD. Efficient identification of these minerals is crucial for monitoring their impact on soils.
This study compares the capabilities of Landsat-09, ASTER, and Sentinel-2 satellite images in identifying Jarosite, Goethite, Ferrihydrite, Anhydrite, and Gypsum (associated with AMD) using the "Spectral Angle Mapping" (SAM) technique. SAM is a spectral analysis method that classifies materials based on the angle between spectral vectors corresponding to their spectral signatures.
The evaluated satellite images were selected based on their spatial, spectral, and temporal resolution. Their strengths and limitations in detecting the selected secondary minerals were assessed using the SAM technique in ENVI software. The algorithm was trained with spectral signatures ranging from 0.4 to 2.5 micrometers, obtained from the USGS and ASTER spectral libraries. Landsat-09 offers moderate resolution and global coverage; ASTER excels in shortwave infrared capabilities but lacks recent satellite imagery for current analyses; and Sentinel-2 combines high resolution with a broad spectral range and biweekly temporal resolution, with continuous image acquisition to date.
The results show significant differences in each sensor's ability to identify the minerals of interest. Sentinel-2 demonstrated high accuracy due to its spatial resolution and specific spectral bands. Conversely, ASTER was unable to precisely delineate pixels associated with the requested minerals. Lastly, Landsat-09 showed limitations in mineral identification using this technique due to the sensor’s spatial resolution. This study highlights that spatial resolution is the most critical factor in selecting satellite imagery for SAM applications. Thus Sentinel-2, with the highest spatial resolution (10 m) achieved superior results in identifying AMD-related minerals.
This study provides guidance for selecting satellite sensors based on spatial and spectral resolutions in studies aimed at mineral identification using SAM. It contributes to the development of more efficient strategies for environmental management, mineral exploration, and energy resource studies, among other applications.

How to cite: Almazan Valencia, J. T., Archundia Peralta, D., and Ramírez Serrato, N. L.: Evaluation of different types of satellite images for the identification of minerals formed by Acid Mine Drainage using Spectral Angle Mapping (SAM), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7570, https://doi.org/10.5194/egusphere-egu25-7570, 2025.

EGU25-8117 | Posters on site | GI6.2

Sea fog detection from GK2A AMI and GK2B GOCI-II satellite images using swin transformer 

Jonggu Kang and Yangwon Lee

Sea fog detection is a critical aspect of meteorological monitoring due to its significant impact on maritime safety and navigation. However, accurately detecting sea fog poses challenges due to its dynamic nature and the limitations of conventional detection methods. Recent advancements in remote sensing technology and deep learning provide an opportunity to overcome these challenges. This study leverages the capabilities of Korea’s geostationary satellites, GK2A AMI and GK2B GOCI-II, and applies a state-of-the-art deep learning model, Swin Transformer-based UPerNet, to develop an efficient sea fog detection system. To achieve this, satellite images from AMI and GOCI-II were collected, preprocessed, and labeled using manual and automated methods. Composite images, generated from selected spectral bands effective for fog detection, served as inputs to the model. The datasets were augmented and standardized to enhance model performance and generalization. The trained model was evaluated using metrics such as overall accuracy (ACC) and critical success index (CSI), achieving 98.8% ACC and 78.76% CSI, respectively, on the test dataset. The results demonstrate the potential of the proposed approach to improve sea fog detection, with applications extending to operational meteorology and maritime safety. Although limitations such as minor distortions in detection accuracy were observed, these can be addressed in future studies by incorporating more advanced models and additional data sources. This research highlights the synergy between geostationary satellite data and deep learning for environmental monitoring and provides a foundation for further advancements in remote sensing applications.

 

This research was supported by a grant (2021-MOIS37-002) of "Intelligent Technology Development Program on Disaster Response and Emergency Management" funded by Ministry of Interior and Safety (MOIS, Korea).

How to cite: Kang, J. and Lee, Y.: Sea fog detection from GK2A AMI and GK2B GOCI-II satellite images using swin transformer, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8117, https://doi.org/10.5194/egusphere-egu25-8117, 2025.

EGU25-9725 | ECS | Posters on site | GI6.2

Seasonal Bias in OCO-2 XCO2 Satellite Observations 

Tslil Nacson, David Broday, and Fadi Kizel

Accurately monitoring atmospheric carbon dioxide (CO₂) is vital for understanding global carbon fluxes and shaping climate mitigation policies. This study explores the seasonal variability of biases between satellite-derived OCO-2 XCO₂ observations and ground-based TCCON XCO₂ measurements at the Caltech TCCON station over nine years (2014–2023). The study categorized the data by observation mode (nadir or glint) and month and investigated the distributions of deviations from the mean bias.

Distinct seasonal patterns emerged in the bias variability. Nadir mode observations demonstrated consistent median deviations, ranging from -0.6 to 0.4 ppm, indicating minimal bias variability. In contrast, glint mode observations showed substantial variability, with absolute median deviations surpassing 1 ppm during January, March, and September. Skewness analysis revealed asymmetries in the data distributions and the presence of significant outliers. A strong correlation was observed between monthly Normalized Difference Vegetation Index (NDVI) values and glint mode skewness (R² = 0.76), highlighting its sensitivity to surface reflectance and vegetation dynamics. In comparison, nadir mode skewness demonstrated greater stability with minimal correlation to NDVI.

The study underscores the need to consider environmental factors, such as vegetation coverage and observation mode differences when interpreting OCO-2 data. By identifying the role of seasonal variability in satellite-ground measurement discrepancies, these findings contribute to refining retrieval algorithms and enhancing satellite-based XCO₂ monitoring accuracy. Improved accuracy supports the development of more reliable carbon flux models, which are essential for effective climate policy and mitigation strategies. Future studies should replicate this analysis at other TCCON stations and incorporate additional environmental variables to further elucidate the drivers of seasonal biases in OCO-2 observations.

How to cite: Nacson, T., Broday, D., and Kizel, F.: Seasonal Bias in OCO-2 XCO2 Satellite Observations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9725, https://doi.org/10.5194/egusphere-egu25-9725, 2025.

EGU25-10367 | ECS | Posters on site | GI6.2

Application of UAV surveys and GIS to investigate factors affecting recreational trail width  

Tweneboah Kodua Dwamena, Marek Ewertowski, and Aleksandra Tomczyk

Monitoring and managing recreational trails are necessary to promote recreation and conservation of protected natural areas (PNAs). However, the relationship between the usage of recreational trails and its impact on the immediate environment can be complex, where a small increase in number of visitors can cause significant damage, or conversely, intensive usage of recreational trails could have a very minimal impact due to other factors like management practices, trial design, the behaviours of users, soil type and resilience make it a non-linear relationship. This research seeks to assess and investigate the relationship between recreational trail width and several morphometric parameters of the trail and its vicinity (e.g., trail gradient, trail aspect, landform gradient, landform aspect, and topographic wetness index). The main aim of this study is to use geographic information systems (GIS) and unmanned aerial vehicle (UAV) data to produce consistent morphometric information about trail conditions. We present a step-by-step workflow demonstrating how to use orthomosaic and digital elevation models (DEMs) generated from UAV surveys to delimitate trail tread and subsequently provide data on trail width, gradient and aspect in a semi-automatic, objective way. The deliverable of our work is a toolbox for ArcPro, which can be implemented to generate trail and terrain characteristics in any area for which trail tread polygon and DEM are provided. Analysing relationships between trail width and other morphometric parameters will help understand factors affecting trail conditions. This study is supported by Polish National Science Center project OPUS-22 2021/43/B/ST10/00950.

How to cite: Dwamena, T. K., Ewertowski, M., and Tomczyk, A.: Application of UAV surveys and GIS to investigate factors affecting recreational trail width , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10367, https://doi.org/10.5194/egusphere-egu25-10367, 2025.

EGU25-11514 | ECS | Orals | GI6.2

Advancements in landslide monitoring by leveraging satellites observations using Offset Tracking algorithms 

Vincenzo Critelli, Melissa Tondo, Cecilia Fabbiani, Marco Mulas, Francesco Lelli, Tommaso Simonelli, and Alessandro Corsini

Satellite remote sensing techniques have emerged as crucial tools in monitoring and analysing Earth's surface, enabling insights into high-risk natural phenomena and enhancing decision-making processes. The PARACELSO project (funded by ASI – Italian Space Agency) aims to leverage satellites observations and innovative data analysis approaches to improve the mapping and surveillance practices of the Po River Basin Authority with respect to the dynamics of rivers, landslides and rock glaciers. As of landslides, the project aims to introduce the usage of techniques such as interferogram stacking and offset tracking (OT) for detecting and monitoring large-scale slope movements characterized by displacement rates higher than these allowing the application of multi-interferometric techniques. In such framework, and with reference to moderate velocity active earthslides and earthflows in the northern Apennines of Italy, this presentation deals with the application of OT algorithms implemented in Python (such as Normalized Cross-Correlation, Phase Correlation and Optical Flow), to imagery from the Sentinel 2 (multispectral), Prisma (hyperspectral) and Cosmo-SkyMed (X-band SAR) missions. Results obtained so far, validated by ground-based evidences and monitoring, confirm that offset tracking can become a powerful tool for leveraging satellite data for characterizing landslide dynamics over both short and extended periods of time. Furthermore, they evidence some limitations and the need for an optimization of data pre-processing routines (e.g., co-registration and terrain correction) and of the OT algorithms (so to reduce computing times). On such basis, it is concluded that using OT algorithms with satellite imagery can effectively allow the extraction of relevant motion distribution at the slope scale for specific landslides and, possibly, allow the identification of unrecognized active phenomena over quite large areas, so to advance the possibility of slope movements detection for hazard and risk management both for researchers and decision-makers.

How to cite: Critelli, V., Tondo, M., Fabbiani, C., Mulas, M., Lelli, F., Simonelli, T., and Corsini, A.: Advancements in landslide monitoring by leveraging satellites observations using Offset Tracking algorithms, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11514, https://doi.org/10.5194/egusphere-egu25-11514, 2025.

EGU25-11516 | ECS | Orals | GI6.2

Historical mapping of fragmented cropland in Africa: a case study in the Copperbelt region, DRC (2000-2023) 

Xiaojing Ou, Pu Shi, Basile Bazirake Mujinya, and Kristof Van Oost

Precise and dynamic cropland maps are essential for research and practical applications, such as soil fertility assessment and crop production monitoring. In Africa, continued population growth and increasing land-use pressures make the need for reliable land cover information greater than ever. Earth observation missions provide timely, large-scale data, and recent efforts have produced high-resolution (30m or better) global and continental cropland/land use land cover (LULC) maps. However, low consensus among these maps for cropland predictions in Africa largely limits their downstream local applicability despite reported high accuracy.

Here, we conducted a case study in the Copperbelt region (DRC), where most cropland is managed by smallholders within fragmented landscapes. Our objectives were to: (i) map cropland dynamics from 2000 to 2023; (ii) evaluate the accuracy of both static maps and dynamic changes (cropland gain and loss); and (iii) compare the performance of our maps with five existing high-resolution (10/30m) cropland/LULC products. We used the Landsat Analysis Ready Data (ARD, 30m resolution) to derive eight annualized NDVI time series (aggregated every three years from 2000 to 2023) as input data. A binary random forest classifier was trained on over 6000 cropland and 12000 non-cropland reference samples collected from 2000 to 2023. Independent validation for the static map in 2020 showed an overall accuracy (OA) of 91.2%, outperforming all existing maps (OA: 60.2%–83.2%). While effective at identifying large cropland fields, most existing maps overlooked small, fragmented fields, leading to an underestimation of cropland area up to 91%. Based on our predicted maps, cropland area increased by 20% from 2000 to 2023. Two drastic short-term changes were observed: a surge from 2017 to 2020 (+57%) and a decrease from 2020 to 2023 (-37%), reflecting intense deforestation and urban expansion in the two periods. However, accuracy for detecting cropland gain (71.9%) and loss (53.3%) was limited, likely due to the 30m resolution being insufficient to separate smaller fields, particularly near suburban built-up areas where cropland is often interspersed with single houses.

In conclusion, existing global and continental cropland/LULC maps remain inadequate for regional use in Africa, where fragmented cropland is prevalent. Improving these maps requires region-specific training samples, particularly from smallholder farms. Moreover, detecting cropland changes remains challenging, and higher-resolution imagery may present an opportunity to better monitor the dynamic landscapes.

How to cite: Ou, X., Shi, P., Bazirake Mujinya, B., and Van Oost, K.: Historical mapping of fragmented cropland in Africa: a case study in the Copperbelt region, DRC (2000-2023), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11516, https://doi.org/10.5194/egusphere-egu25-11516, 2025.

EGU25-12963 | ECS | Orals | GI6.2

A tool to extract coastlines and shore buffer zones using satellite imagery and Google Earth Engine 

Pilar Martín-Gallego, Juan Montes, Irene Delgado-Fernandez, Laura Del Río, and Christopher Marston

Assessment of shoreline evolution is key for many coastal management and practical applications. Coastal zones are dynamic by nature, with this dynamism subject to numerous studies often focusing on the identification of ‘coastlines’/’shorelines’. Where this coastline (or shoreline) location is, and how it changes, is a fundamental variable in understanding coastal environments. For example, beaches are highly mobile and their interaction with coastal dunes has been key for the development of classical conceptual models. A number of remote sensing methods and algorithms have been designed to extract instantaneous coastlines from satellite imagery. These represent a snapshot of the position of the coastline at a particular time. However, coastlines do not exist over a time period, as they dissolve in a ‘buffer zone’, an interphase between land and ocean where water and sand are constantly mixing. This buffer zone can vary in size depending on the location and the time of the year. Drawing on the experience gathered by the use of variance images from Argus video monitoring systems, we present an alternative approach for coastline and shore buffer zone detection using medium resolution satellite imagery and Google Earth Engine. This method takes advantage of the increasing availability of satellite data and focuses on collections of satellite images acquired over time periods, instead of single-date images. It aims to minimise user input by applying image compositing and segmentation, with shore buffer zones identified using variance image composites. The approach is tested in beaches with diverse hydro and morphodynamic characteristics. This method obtains medium to long term information of coastal dynamics including average coastline locations and extent of shore buffer zones.

How to cite: Martín-Gallego, P., Montes, J., Delgado-Fernandez, I., Del Río, L., and Marston, C.: A tool to extract coastlines and shore buffer zones using satellite imagery and Google Earth Engine, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12963, https://doi.org/10.5194/egusphere-egu25-12963, 2025.

Land degradation is a key threat to the productivity of agroecosystems which are increasingly pressured by climate change and growing global populations. Land degradation can impact arable land through a range of pathways including physical processes such as salinization and erosion, loss or inhibition of biological function in soils through chemical or physical deterioration, and through climatic shifts such as aridification which are projected to worsen in coming decades. Land degradation affects a large but uncertain portion of agricultural land globally and the implication of degradation for food production is highly variable. Despite the widely recognized prevalence of cropland degradation and its potential impacts, tools for measuring and monitoring productivity losses over long time periods and large spatial scales are lacking. Many global maps of land degradation rely on outdated statistics, manual surveys, and overly basic image analysis and computational approaches. Existing land degradation assessments also lack the granularity required for decision-making at regional and local levels. The robust spatial and temporal availability of remote sensing imagery presents a unique opportunity to monitor the long-term trends in productivity of cropland through measurements of vegetation greenness as a proxy for yield. In this work, we present a novel methodology for detecting long-term changes in cropland productivity that is globally scalable and robust to changes in land use and management. Using the entire MODIS imagery record (2000-2024), we use a Discrete Wavelet Transform to decompose EVI signals and isolate the long-term trend in vegetation greenness at 250m resolution for a test region covering Argentinian croplands. We find that large areas of maize and soy cropland in Argentina have a negative trend in long-term greenness, with subtle but important long-term declines in productivity that may be attributable to degradation. These declines appear more pronounced in older croplands than in newer croplands suggesting a potential cause in soil health related changes. The approach presented is globally applicable and advances the use of earth observation technology to measure land degradation and monitor land use change. 

How to cite: Ippolito, T., Neff, J., Campos, A., and Romero, D.: Remote Sensing-based Detection of Cropland Degradation Signals Using Discrete Wavelet Decomposition Analysis – A Case Study in Argentina , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13096, https://doi.org/10.5194/egusphere-egu25-13096, 2025.

EGU25-13838 | Orals | GI6.2 | Highlight

New Environmental Measurement and Monitoring with 120,000 EMIT Imaging Spectroscopy Scenes Acquired Across Six Continents from the International Space Station. 

Robert Green, David Thompson, Philip Brodrick, Dana Chadwick, and Andrew Thorpe

The prime mission of the Earth Surface Mineral Dust Source Investigation (EMIT) was to characterize the mineral composition of the Earth’s arid land regions, deliver new constraints on the radiative forcing impacts of mineral dust aerosols in the Earth System today, and assess potential changes in the future. To achieve this objective, a high signal-to-noise ratio imaging spectrometer measuring the visible to short wavelength infrared (VSWIR) was developed and then launched to the International Space Station (ISS) on the 14th of July 2022. Having measured more than 100 billion spectra across six continents, EMIT reported prime mission success on the 26th of August 2024. Also in 2024, the EMIT mission was extended and the target observation areas expanded to include biodiversity, terrestrial ecology, corals, volcanos, coastal and inland waters, mid/low latitude snow/ice, and new geology regions across the six continents observable from the ISS.  In addition to new science, these extended mission observations support a broad set of new measurement and monitoring applications related to agriculture, forestry, critical minerals, water quality, wildfire fuels and burn severity, water resources, surface plastics, and more. In support of these objectives, >120,000 EMIT VSWIR imaging spectroscopy scenes have been measured and are currently available as radiance and reflectance along with a suite of mineralogy products. A new fractional cover product with photosynthetic vegetation, non-photosynthetic vegetation, soil, snow/ice, water, and char is in development. All EMIT data and products are freely available from the NASA Land Process Distributed Active Archive Center (LP DAAC). EMIT measurements and products include uncertainty estimates, and the project algorithms are available on GitHub. This contribution on remote sensing environmental monitoring presents new results from EMIT observations along with an overview of the measurements, products, and plans for the ongoing mission. EMIT observations also support preparatory activities for NASA’s Surface Geology and Biology Decadal Survey mission with a next-generation VSWIR imaging spectrometer that is part of the NASA Earth System Observatory and a companion mission to ESA’s Copernicus Hyperspectral Imaging Mission for the Environment (CHIME).

 

How to cite: Green, R., Thompson, D., Brodrick, P., Chadwick, D., and Thorpe, A.: New Environmental Measurement and Monitoring with 120,000 EMIT Imaging Spectroscopy Scenes Acquired Across Six Continents from the International Space Station., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13838, https://doi.org/10.5194/egusphere-egu25-13838, 2025.

EGU25-14722 | Orals | GI6.2

Development of a ground-based microwave spectral radiometer - a downsized version of the satellite-mounted SAMRAI 

Takashi Maeda, Yuta Kobayashi, Nguyen Tat Trung, Yoh Takei, Tsutomu Yano, and Naoya Tomii

Scanning Array for hyper-Multispectral RAdiowave Imaging (SAMRAI) is a passive interferometric radiometer. In this respect, it is similar to MIRAS on board the SMOS satellite launched by ESA, but it realizes ultra-wideband (1-41 GHz) and high-frequency-resolution (27 MHz) microwave spectrum measurement. We believe that SAMRAI is the world's first microwave hyperspectral radiometer.

JAXA will continue to operate the satellite-borne microwave radiometer AMSR series for more than 30 years, including AMSR3 currently under development. The design has remained largely unchanged for 30 years, and various issues are becoming apparent. In particular, the radio frequency interference (RFI) contaminating the natural-origin signals is a serious problem, and we believe that microwave hyperspectral measurement is essential for identifying and isolating RFI signals. This was a big motivation for developing SAMRAI. In addition, microwave hyperspectral measurement must have new possibilities, such as making it possible to measure the frequency characteristics of the emissivity of the Earth surface.

Development of the satellite-borne SAMRAI is progressing toward launch in 2027. On the other hand, as the microwave spectrum from the Earth surface will be observed from a satellite for the first time in the world, pre-launch calibration and validation activities are more important than ever in order to generate geophysical data promptly after the satellite is launched. From this perspective, we have developed a ground-based microwave spectral radiometer using part of the SAMRAI receiver system. This ground-based microwave spectral radiometer is much smaller than SAMRAI and can be easily taken out to various environments for observation, and like SAMRAI, it is capable of measuring microwave spectra at 27 MHz intervals from 1 GHz to 41 GHz.

Here, we presents the technical detail of this ground-based microwave spectral radiometer and its performance confirmation results of the observation experiment in addition to the current status of the satellite-mounted SAMRAI development.

How to cite: Maeda, T., Kobayashi, Y., Tat Trung, N., Takei, Y., Yano, T., and Tomii, N.: Development of a ground-based microwave spectral radiometer - a downsized version of the satellite-mounted SAMRAI, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14722, https://doi.org/10.5194/egusphere-egu25-14722, 2025.

EGU25-15180 | ECS | Posters on site | GI6.2

Satellite-Based Quantification of Temporal Changes in Mine Areas and their Environmental Footprint 

Vincent Nwazelibe, Weikang Yu, Richard Gloaguen, Moritz Kirsch, Raimon Tolosana-Delgado, and Samuel Thiele

Environmental, Social, and Governance (ESG) principles are critical for improving sustainable mining practices and ensuring mining accountability in mitigating environmental and social impacts. Geometallurgy enhances the efficiency of resource extraction and processing by integrating geological, mineralogical, and metallurgical data throughout exploration and operational phases. Mining operations can contribute to ESG goals, decrease waste, and maximise resource utilisation by identifying temporal changes in mine surface features and their environmental impacts for optimisation. These impacts arise from processes throughout the mine life cycle, requiring continuous monitoring of mine expansion and environmental footprint. Hence, predicting the feasibility of a mining project as early as possible is crucial to minimising the impact of exploration activities and avoiding later failures that could have been anticipated. To this purpose, we develop a strategy to include ESG aspects as early as possible in addition to the now common geometallurgical aspects. This study integrates a range of satellite sources (SPOT 1-5, Landsat 5-9, Sentinel-2, and high-resolution Google Earth imagery) to quantify temporal changes in mine surface features across four mines (Vametco, Mogalakwena, Trident, and Gamsberg) representing diverse commodities (vanadium, platinum, copper, and zinc) and identify environmental impact trends for assessment and planning. We manually mapped key mine features, such as pits, overburden waste dumps, tailing dams, slag dumps, stockpiles, and processing areas. Using deep learning methods, we used mine features as training data to explore temporal multiclass change detection with multisource satellite data. We compare the manually mapped results with the deep learning methods and analyse correlations across mine sections, focusing on lateral expansions of mine surface features rather than vertical or depth expansions. Additionally, we assess how mine operations affect environmental components like vegetation, land use, and carbon emissions. Our results demonstrate the usage of satellite data for cost-effective mine monitoring to improve transparency and support compliance with ESG guidelines.

How to cite: Nwazelibe, V., Yu, W., Gloaguen, R., Kirsch, M., Tolosana-Delgado, R., and Thiele, S.: Satellite-Based Quantification of Temporal Changes in Mine Areas and their Environmental Footprint, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15180, https://doi.org/10.5194/egusphere-egu25-15180, 2025.

The Bidirectional Reflectance Distribution Function (BRDF) quantifies the reflected light from a surface as a function of illumination and observation angles. It is a crucial yet challenging aspect of remote sensing, essential for characterizing surface reflectance and properties. Accurate BRDF measurements are integral to surface property analysis and various remote sensing applications. Conventional methods, such as goniometers, provide precise angle-dependent evaluations. However, their high cost, bulkiness, and limited portability significantly hinder their deployment in diverse real-world scenarios. Alternatively, free-handed BRDF measurement techniques eliminate fixed setups but suffer from human error and subjectivity, leading to inconsistent results.

We propose a novel automated system combining a robotic arm and spectral sensors to address these limitations. The system utilizes a robotic arm to precisely maneuver the sensor on a hemispherical trajectory around the target surface, ensuring consistent angles and distances throughout the measurement process. Specifically, the UR10e robotic arm by Universal Robots, with its 12.5 kg payload, 1300 mm reach, and six flexible joints, was employed for its precision, flexibility, and advanced motion control capabilities.

Programming the robotic arm for BRDF measurements required solving a constrained generalized inverse kinematics problem optimized using fuzzy logic to ensure collision-free movement and clear sensor fields of view. Experimental validation demonstrated exceptional sensor localization accuracy, achieving an angular precision of 0.1° under optimal conditions. This automated system facilitates spectral BRDF measurement and modeling across various surfaces with enhanced accuracy, speed, and operational feasibility.

Once the method is fully validated under controlled laboratory conditions, we intend to extend the application of this system to outdoor, real-life scenarios. The robotic arm will be mounted on a platform to conduct measurements in natural environments. This next step aims to evaluate the system's robustness and effectiveness in capturing BRDF data under varying environmental conditions, ultimately confirming its suitability for real-world applications. Such advancements will significantly enhance the accuracy and practicality of BRDF measurements for diverse industries and research domains.

How to cite: Amir, A. and Kizel, F.: A Novel Approach for Automatically Measuring the Bidirectional Reflectance Distribution Function (BRDF) of Surfaces Using Spectral Sensors and a Robotic Arm., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15542, https://doi.org/10.5194/egusphere-egu25-15542, 2025.

Earth's surface, our primary habitat, provides essential ecosystem and social services, such as carbon sequestration and food production. Numerous studies reveal that global changes are destabilizing the Earth's surface, as evidenced by extreme events' increasing frequency and complexity. These events trigger substantial losses across various sectors, including the economy and public health, necessitating accurate detection. Currently, large-scale monitoring of phenomena like vegetation disturbances and wildfires is achieved using remote sensing, with detection accuracy expected to improve through advanced machine learning techniques. However, these approaches primarily provide specific, event-based information, detecting only predefined types of events. Macroscopic mapping, which involves identifying these instabilities without relying on specific event types, remains unresolved despite its value for comprehensive detection and broader understanding.

To fill this gap, we propose a novel method for detecting unstable surfaces, termed Surface Anomalies (SAs). We hypothesize that a surface's evolution is influenced by its initial state and environmental factors within a given geographical region, including climate and land use. Consequently, homogeneous surfaces with similar initial states under comparable environmental conditions are expected to follow similar evolutionary trajectories. Building upon this hypothesis, SAs are defined as surfaces with evolutionary trajectories that deviate from their homogeneous counterparts. Compared to event-based definitions, our conceptual framework accommodates instabilities that are not predefined yet are nonetheless important, providing more comprehensive detection. Compared to algebraic change or anomaly detection methods, our definition offers a more precise characterization of SAs and has the potential to reduce irrelevant detections.

We operationalize this conceptual framework using remote sensing imagery in a two-stage process. In the first phase, we model the normal evolutionary patterns of a region. This involves acquiring a pair of baseline images where each pixel represents a surface, spectral values represent surface states, and differences between images represent evolutionary trajectories. We apply K-Means clustering with a sufficiently large number of cluster centers to segment the imagery, with each cluster corresponding to a type of homogeneous surface. For each homogeneous surface, we fit a Gaussian Mixture Model to the distribution of evolutionary trajectories, representing normalcy. In the detection phase, we acquire new image pairs from nearby locations and calculate the probability that their evolutionary trajectories fit within the GMM of the corresponding homogeneous surface model. Lower probabilities indicate higher instability. This probabilistic approach allows us to detect surface anomalies by identifying deviations from normal evolutionary patterns.

We evaluated our method's effectiveness by comparing it with traditional non-event-based approaches such as algebraic change detection and change vector analysis. This comparison was performed on a dataset encompassing various types of SAs, including wildfires, floods, volcanic activities, deforestation, and bark beetle infestations. Our method's results indicate significant improvements, substantially reducing false alarms and omissions. In summary, our method for detecting SAs from a macroscopic perspective has the potential to enhance our understanding of how Earth's surface responds to global change.

How to cite: Xu, J., Yan, K., and Wang, Q.: Dynamic Modeling Reveals Earth Surface Anomalies: An Innovative Conceptual Framework and Detection Method, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15649, https://doi.org/10.5194/egusphere-egu25-15649, 2025.

EGU25-15819 | ECS | Posters on site | GI6.2

Long term ground deformation analysis of landslide integrating remote sensed and in-situ data 

Olga Nardini, Francesco Poggi, Matteo Del Soldato, Silvia Bianchini, and Chiara Scaini

Landslides represent a significant natural hazard on a global scale, resulting in considerable economic losses and indirect social impacts. Italy is one of the European countries most affected by landslides, with more than 500,000 mapped events, of which approximately 100,000 are located in Tuscany. Remote sensing has emerged as a powerful tool for the investigation and monitoring of ground deformation. Earth observation techniques, particularly the Interferometric Synthetic Aperture Radar (InSAR) analysis and optical imagery enable ground deformation measurement with millimetric to centimetric precision and high temporal frequency.

The present study focuses on the municipality of Zeri, in the province of Massa-Carrara (Tuscany), specifically on the hamlets of Patigno and Coloretta affected by quiescent and active landslides. These areas have been selected considering the displacement recorded by the Interferometric Synthetic Aperture Radar (InSAR) data from Sentinel-1 for the period 2019-2023. Data is made available from the European Ground Motion Service (EGMS), enabling precise measurements of ground deformation over time with millimetric accuracy through the time-series analysis. For this reason, Zeri municipality was chosen as a case study for exploring the interplay between optical and radar satellite-derived deformation data and in-situ information on buildings impacted by landslides. A multi-temporal analysis integrating advanced remote sensing techniques employs optical imagery, acquired from high-resolution sensors such as WorldView-2/3, SPOT-7, and other oldest aerial optical datasets, to provide long-term information on surface changes, vegetation displacement, and impact of the landslides on the structures and infrastructure.

The integration of these datasets allows for a comprehensive assessment of the spatial and temporal evolution of ground movements, highlighting areas of active deformation and their direct impact on built structures. By correlating both radar and optical satellite-derived deformation trends with detailed in-situ surveys of buildings, the study aims to identify patterns of structural vulnerability and the progression of damage linked to ongoing ground instability. This dual approach leverages the strengths of optical and SAR data to enhance the understanding of landslide dynamics in this geologically complex area, providing a robust basis for further risk assessment and mitigation planning.

The research is part of the PRIN-PNRR project SMILE: Statistical Machine Learning for Exposure development, funded by the European Union- Next Generation EU, Mission 4 Component 1 (CUP F53D23010780001), which aims to investigate how Machine Learning (ML) can be used to assemble or update exposure layers by combining crowdsourced data gathered by trained citizens, ancillary data (such as national census data), and remote sensing images.

How to cite: Nardini, O., Poggi, F., Del Soldato, M., Bianchini, S., and Scaini, C.: Long term ground deformation analysis of landslide integrating remote sensed and in-situ data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15819, https://doi.org/10.5194/egusphere-egu25-15819, 2025.

EGU25-18572 | Posters on site | GI6.2

Practical guidelines for performing UAV  mapping flights  

Wouter Maes

Uncrewed Aerial Vehicles (UAVs) have transformed remote sensing, offering unparalleled flexibility and spatial resolution across diverse applications. Many of these applications rely on mapping flights using snapshot imaging sensors, for creating 3D models of the area, or for generating orthomosaics from RGB, multispectral, hyperspectral or thermal cameras. Based on a literature review,  comprehensive guidelines for executing mapping flights for the different sensors are here formulated, addressing flight preparation, planning and execution. Key considerations in flight preparation and planning covered include sensor selection, flight altitude and GSD, flight speed, overlap settings, flight pattern, direction and viewing angle; considerations in flight execution include on-site preparations (GCPs, camera settings, sensor calibration and reference targets) as well as on-site conditions (weather conditions, time of the flights) to take into account. In all these steps, high-resolution and high-quality data acquisition needs to be balanced with feasibility constraints such as flight time, data volume and post-flight processing time. The formulated guidelines are based on literature consensus. However, knowledge gaps for mapping flight settings are identified, particularly in flight direction and for thermal imaging in general. These guidelines and identified knowledge gaps are useful to advance the harmonization of UAV mapping practices, promoting reproducibility and enhanced data quality across diverse applications.

How to cite: Maes, W.: Practical guidelines for performing UAV  mapping flights , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18572, https://doi.org/10.5194/egusphere-egu25-18572, 2025.

EGU25-18858 | ECS | Posters on site | GI6.2

Evolution of Inland Water Bodies in Summer and Their Response to Heatwaves: A Case Study of Shaanxi Province in China 

Meiling Gao, Ying Wen, Jie Li, Zhenyu Tan, and Zhenhong Li

The evolution of Inland Water Area (IWA) is strongly influenced by climate change. Against the backdrop of frequent extreme heat events in recent years, the impact of summer heat on IWA warrants further attention. Using the Google Earth Engine platform and integrating multi-source remote sensing data, this study developed a refined identification scheme capable of effectively capturing small inland water bodies. Then, the linear slope and coefficient of variation were used to reveal the spatio-temporal variation characteristics of IWA at county scale in Shaanxi Province during the summer seasons from 2016 to 2022. Subsequently, coupled with the estimated daily maximum temperature data, the spatio-temporal correlation between summer heat and IWA was quantified by applying Pearson correlation coefficient and the global Moran's index. Finally, the driving process of summer heat on IWA was explored by using Geodetector and geographical weighted regression model in conjunction with various natural factors. The results show that: (1) The overall accuracy of the inland water body identification scheme developed in this study is 0.967, with the Kappa coefficient of 0.924. The spatial distribution of inland water bodies in Shaanxi Province during the study period is uneven, with higher fluctuations in areas with fewer water bodies. And there is an overall increasing trend in the spatio-temporal variation of IWA. (2) The spatial and temporal correlations between heat indices represented by TXx, TX5d, TX7d, TX10d, TX15d, and TX90p and IWA are all negatively correlated. The highest correlation was observed between TX10d and IWA, with a Pearson correlation coefficient of -0.812 and a Global Moran’s I of -0.173. (3) The summer heats in Shaanxi Province negatively inhibit IWA, with regression coefficients ranging from -0.110 to -0.483. In addition, the dry areas with fewer IWA in northern Shaanxi and flatter terrains in Guanzhong are susceptible to summer heat inhibition. Moreover, the absolute values of the regression coefficients between TX10d and IWA gradually decreased from the arid, low-precipitation climate of northern Shaanxi to the humid, high-precipitation climate of southern Shaanxi, indicating that the arid climate and insufficient precipitation will magnify the inhibitory effect of summer heat, whereas the humid climate and abundant rainfall will alleviate the negative effect of summer heat. On the other hand, surface runoff showed the positive effect on IWA, with regression coefficients ranging from 0.110 to 0.449. Climate warming induces an increase in surface runoff, which is conducive to the expansion of IWA. This study provides a scientific reference for the rational planning and management of surface water resources under climate warming scenarios.

How to cite: Gao, M., Wen, Y., Li, J., Tan, Z., and Li, Z.: Evolution of Inland Water Bodies in Summer and Their Response to Heatwaves: A Case Study of Shaanxi Province in China, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18858, https://doi.org/10.5194/egusphere-egu25-18858, 2025.

EGU25-19616 | ECS | Posters on site | GI6.2

Traditional and Unmixing-Based semi-empirical models for BRDF correction in time series data 

Yulia Vidro and Fadi Kizel

This research investigates two methodologies for correcting the Bidirectional Reflectance Distribution Function (BRDF) in Sentinel-2 imagery, focusing on transition zone in Israel between arid and sub-humid climatic zones across a year-long temporal span. BRDF correction is critical in remote sensing applications, especially for multi-temporal analysis, as it accounts for variations in surface reflectance due to changing illumination and viewing geometries. The study aims to compare the performance of these methods in normalizing surface reflectance and minimizing angular effects, enhancing the accuracy of time-series analysis for environmental monitoring. In particular, we test the performance of the traditional semi-empirical kernel-driven BRDF model, namely the Ross-Thick-Maignan (RTM) volumetric kernel and the Li-Transit-Reciprocal (LTR) geometric kernel and a recently proposed correction method RTM-LS-UMx, which relies on the kernel-driven model but incorporates the spectral unmixing results within the inversion process. This method was reported to be advantageous for mosaics of airborne images and laboratory data in previous work. Therefore, we aim to test this technique on satellite images influenced by seasonal changes in the sun’s position. We analyzed images of a transition zone in Israel between arid and sub-humid climatic zones to achieve this. The images were acquired in summer, mid-fall, and winter; thus, the sun’s position at this latitude affects the measured reflectance. Pre-processing steps included radiometric calibration, atmospheric correction, and cloud masking to ensure consistency across datasets. Quantitative evaluation used performance metrics, including the Normalized Difference Vegetation Index (NDVI) stability, Root Mean Square Error (RMSE) against a ground-truth dataset, and angular dependency reduction. Results indicated that both methods significantly improved reflectance consistency compared to uncorrected imagery. However, the unmixing-based model RTM-LS-UMx was advantageous concerning all examined metrics. The study further explored the impact of BRDF correction on long-term environmental monitoring applications. Time-series analysis revealed that both methods enhanced the detection of subtle surface changes previously obscured by angular variations. 

How to cite: Vidro, Y. and Kizel, F.: Traditional and Unmixing-Based semi-empirical models for BRDF correction in time series data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19616, https://doi.org/10.5194/egusphere-egu25-19616, 2025.

EGU25-2144 | PICO | GM2.5

Mapping fractures in 3D from airborne LiDAR: comparison with field mapping 

Sara Carena and Anke Friedrich

We tested whether public high-resolution airborne LiDAR data could be suitable for structural geology applications by comparing fracture orientation measurements on Virtual Outcrop Models (VOMs) to field measurements from the same outcrops. We found that the fundamental requirement for taking full advantage of such data is good bedrock exposure, which is also dependent on lithology. Whenever this requirement is satisfied, VOM measurements are comparable to field measurements. VOMs can help considerably in both reducing the time it takes to collect measurements, and in expanding the area in which measurements can be collected without adding significantly to the time budget. They are also especially useful in remote regions and at high elevations, where access is more difficult and yet good exposures are more likely to be found, and they should always be used when planning field work. At present  the main limitations, apart from LiDAR coverage not yet existing in places, are due to the hardware and software capabilities needed to create and especially to analyze VOMs. 

How to cite: Carena, S. and Friedrich, A.: Mapping fractures in 3D from airborne LiDAR: comparison with field mapping, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2144, https://doi.org/10.5194/egusphere-egu25-2144, 2025.

EGU25-2736 | PICO | GM2.5

Extraction and Orientation Analysis of Rock Mass Discontinuities Using UAV-Assisted Photogrammetry 

Xianquan Han, Ruoming Zhai, Yuewen Huang, and Bangning Ding

The stability of rock masses is crucial for the safety of hydraulic engineering, as the integrity of the rock mass directly influences the stability of structures such as dams, reservoirs, and tunnels. Accurate extraction and orientation of rock mass discontinuities plays a key role in stability analysis, providing essential geometric data for assessing rock mass behavior. However, traditional manual measurement methods used to extract these orientations are not only time-consuming and labor-intensive but also fraught with safety risks, especially when working on large and steep slopes. These limitations hinder the efficiency and accuracy of rock mass stability assessments.

To address these challenges, this paper proposes a novel approach for acquiring 3D rock mass scenes using unmanned aerial vehicles (UAVs), coupled with oblique photogrammetry technology for 3D scene reconstruction. With UAVs equipped with high-resolution cameras to capture image sequences from various angles, the Structure from Motion (SfM) algorithm is then applied to reconstruct the 3D scene. This method allows for the generation of high-precision point cloud data through geometric uniform sampling, ensuring accurate representation of rock mass. Once the 3D scene is reconstructed, local geometric features (including surface curvature, planarity, scattering, and verticality) are calculated based on neighborhood search. Combined with RGB texture information, machine learning method is employed to analyze the importance of these features, and further identify and differentiate rock mass features from vegetation and outliers within the large-scale slope scene, followed by a region-growing and merging algorithm for the segmentation of rock mass patches. For each individual patch, a local planar coordinate system is established to generate a grayscale image, which is then used for edge detection to identify structural boundaries. Following this, line extraction is carried out using an energy-optimization-based graph cut algorithm, and the closed contours of the structural patches are delineated through vectorization, ensuring an accurate and detailed mapping of the rock mass structure.

The effectiveness of the proposed method was validated through experiments conducted on a large-scale rock mass slope scene. The results demonstrate that the method can accurately extract the rock mass structural regions, identify the fracture network, and provide crucial geometric features, such as dip, strike, and trace information for each structural plane. The extracted features significantly contribute to evaluating the structural integrity and stability of large-scale slopes, offering a more efficient, accurate, and safer alternative to traditional manual measurement methods. Moreover, this method can be applied to a wide range of geological environments, providing a valuable tool for real-time monitoring and assessment in engineering projects.

How to cite: Han, X., Zhai, R., Huang, Y., and Ding, B.: Extraction and Orientation Analysis of Rock Mass Discontinuities Using UAV-Assisted Photogrammetry, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2736, https://doi.org/10.5194/egusphere-egu25-2736, 2025.

EGU25-4331 | PICO | GM2.5

An Introduction to Fully Automated Co-Alignment - FACA 

Nick Schüßler, Jewgenij Torizin, Claudia Gunkel, Michael Fuchs, Karsten Schütze, Lars Tiepolt, and Dirk Kuhn

Well-aligned point cloud time series data generated with Unmanned Aerial Vehicles (UAVs) can be a significant asset to geoscientists.
Practitioners benefit from multi-temporal point clouds with high comparative accuracy, e.g. to evaluate landscape changes after landslides and quantify mass wasting.
Two approaches are usually applied to achieve the accurate alignment of point clouds: indirect and direct georeferencing.
Indirect georeferencing uses well distributed Ground Control Points (GCPs) in the study area.
While this method significantly enhances the precision and accuracy of time series point clouds, the placement and measurement of GCPs are time-intensive and may even be impossible in difficult terrain.
Direct georeferencing depends on highly precise and accurate location information embedded in images, which is often viable only with expensive real-time kinematic (RTK) positioning equipment or post-processed kinematic (PPK) services.
Beyond the extra cost, this approach faces the same challenges as indirect georeferencing, particularly in the placement of equipment and scalability for large areas.

Recent research has introduced an alternative method called Co-Alignment, which enables the alignment of point clouds with high local precision without GCPs and RTK data. Moreover, when GCPs or RTK are used, co-alignment can further enhance accuracy of the point cloud alignment.
This method aligns multiple point clouds with good local precision without requiring GCPs or RTK equipment, though it lacks global accuracy.
The workflow uses common, unchanged features in the study area, such as anthropogenic structures or boulders, to establish spatial references across multiple epochs using computer vision algorithms.

We developed FACA - Fully Automated Co-Alignment to implement the Co-Alignment workflow.
With FACA, we aim to offer easy access to a scalable point cloud alignment method.
FACA is automatable from the command line and user-friendly through a custom graphical user interface, making it adaptable to common point cloud generation workflows.
Released as open-source software under the GNU General Public License v3, FACA is freely accessible and modifiable to meet diverse user requirements.
By integrating with Agisoft Metashape Professional, FACA leverages advanced photogrammetric features to enhance performance and output quality.
We present the FACA workflow, emphasizing its ease of use, scalability, performance, supported by results from data acquired at Germany's Baltic Sea coast and in Svalbard.

Furthermore, we discuss the potential for custom software solutions to further improve and expand the workflow’s capabilities.

How to cite: Schüßler, N., Torizin, J., Gunkel, C., Fuchs, M., Schütze, K., Tiepolt, L., and Kuhn, D.: An Introduction to Fully Automated Co-Alignment - FACA, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4331, https://doi.org/10.5194/egusphere-egu25-4331, 2025.

EGU25-5168 | PICO | GM2.5

Unlocking the potential of historical aerial and spy satellite stereo-imagery in geosciences: access, processing, and applications 

Livia Piermattei, Robert McNabb, Melanie Elias, Camillo Ressl, Amaury Dehecq, Luc Girod, Thomas Dewez, and Anette Eltner

Historical imagery captured from aeroplanes since the early 1900s and from spy satellites from the 1960s onwards have long been used in natural sciences for military, civil, and research purposes. These images have the unequalled potential for documenting and quantifying past environmental changes caused by natural and anthropogenic factors. Especially when acquired in stereo mode, these images enable the generation of point clouds and digital elevation models (DEMs), allowing us to quantify surface elevation changes over the past century.

Recent advancements in digital photogrammetry and the increasing availability of historical photographs as digitised/scanned images have heightened the interest in these data for reconstructing long-term surface evolution from local to regional scale. However, despite the large archive of historical images, their full potential is not yet widely exploited. Key challenges include accessibility, lack of metadata, image degradation, limited resolution and accuracy and lack of standardised workflows for generating DEMs and orthophotos.

We reviewed 198 journal articles published between 2001 and 2023 that processed historical aerial and spy satellite imagery. Our review spans methodological advancements in photogrammetric reconstruction and applied research analysing past 2D and 3D environmental changes across geoscience fields, such as geomorphology, cryosphere, volcanology, forestry, etc. We provide a comprehensive overview of these studies, summarise the image archives, applications, and products, and compare the methods used to process historical aerial and spy satellite imagery. Furthermore, we highlight emerging workflows and offer recommendations for image processing and accuracy assessment for future research and applications.

How to cite: Piermattei, L., McNabb, R., Elias, M., Ressl, C., Dehecq, A., Girod, L., Dewez, T., and Eltner, A.: Unlocking the potential of historical aerial and spy satellite stereo-imagery in geosciences: access, processing, and applications, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5168, https://doi.org/10.5194/egusphere-egu25-5168, 2025.

The project's goal is to create a software tool for detecting and predicting a higher form of (rill) erosion on agricultural land. The planned tool's innovative potential is the use of neural networks on the joint remote sensing and erosion-hydrological modelling data. Morphological parameters and erosion-hydrological causal event response thus enhance common inputs for the neural network-driven semantic segmentation.

By combining morphological parameters, event-based hydrological responses, and a calculated critical water layer thickness (hcrit) from physical SMODERP model - the threshold at which rill erosion begins - the tool enhances the precision of high-risk area delineation, supporting smart agriculture and climate adaptation.

The project utilizes a unique dataset of manually digitized erosion rills from over 20 years of aerial orthophotos, enabling comprehensive training of neural networks. Multi-resolution data, including satellite imagery, aerial orthophotos, and UAV images, are combined to identify and refine morphological properties critical for rill erosion detection. Several types of neural networks were tested, notably FCN, U-Net, SegNet, DeepLabv3+, to evaluate their effectiveness in handling diverse input data and optimizing predictive accuracy. Automated workflows for dataset expansion and retraining ensure adaptability to new data.

Validation of the model will be performed using the original dataset of manually digitized erosion rills as a benchmark for accuracy. By comparing the predicted rill locations with this dataset, the model’s performance can be rigorously evaluated and adjusted. Real-time erosion event mapping, supported by the Agricultural Land Erosion Monitoring system, will complement this process by incorporating contemporary data to further enhance model reliability. This innovative tool addresses gaps in existing methods by combining predictive capabilities with detailed spatial data, improving erosion detection accuracy for sustainable land management under changing climatic conditions.

The research is funded by the Technological Agency of the Czech Republic research project (TQ03000408)- Detection of Increased Erosion Damage Using Neural Networks on a Combination of Remote Sensing Imagery and Erosion-Hydrological Modeling and an internal student CTU grant (SGS23/155/OHK1/3T/11).

How to cite: Tejkl, A., Kavka, P., Pesek, O., and Landa, M.: Detection of Increased Erosion Damage Using Neural Networks on a Combination of Remote Sensing Imagery and Erosion-Hydrological Modeling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5875, https://doi.org/10.5194/egusphere-egu25-5875, 2025.

EGU25-6611 | ECS | PICO | GM2.5

The use of computer vision to relocate historical aerial photographs that enhance the understanding of hydrogeomophic changes in Ethiopia 

Michiel De Baets, Lore Lamote, Jonathan Sterckx, Sofie Annys, Jan Nyssen, Hiep Luong, Tesfaalem Gebreyohannes, and Amaury Frankl

The digitisation of historical aerial photograph archives offers a unique opportunity to analyse long-term environmental changes. One such valuable resource is the archive of 1935-1941 aerial photographs of Ethiopia, one of the largest and oldest collections in Africa, comprising 34,000 images. While a portion of these images has been localized, many remain without known coordinates. To address this, we developed a computer vision approach that combines scale invariant feature transform (SIFT) keypoint matching and nearest-neighbour search, achieving 99% accuracy and 80% recall in matching images. This method increased the localization rate from 40% to approximately 70%, though manual verification and coordinate determination remain necessary. A proof-of-concept further demonstrated the potential of utilizing depth information to localize photographs: by leveraging the spatial proximity of images within the quite erratic flight lines, we significantly reduced the search area. Additionally, we show that 3D scene reconstruction from consecutive images, matched to a digital elevation model using the ICP algorithm, is feasible.

We demonstrate the potential of historical aerial archives for studying long-term environmental change through a case study on river geomorphology. At 70 locations where aerial photographs intersect major unconfined rivers, we analysed key hydrogeomorphological variables to assess river dynamics. By comparing river morphology in 1935-1941 with that on the most recent Google Earth imagery, our results reveal significant morphological changes, including channel widening, gullying, bank erosion, and in-stream sediment accumulation. These findings highlight how a detailed understanding of local river dynamics, derived from historical and modern imagery, can enhance the broader understanding of environmental changes and their impacts on catchment behaviour.

Key words: Aerial Photographs, Environmental Change, Hydrogeomorphology, Environmental Change, River

How to cite: De Baets, M., Lamote, L., Sterckx, J., Annys, S., Nyssen, J., Luong, H., Gebreyohannes, T., and Frankl, A.: The use of computer vision to relocate historical aerial photographs that enhance the understanding of hydrogeomophic changes in Ethiopia, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6611, https://doi.org/10.5194/egusphere-egu25-6611, 2025.

EGU25-6774 | ECS | PICO | GM2.5

Historical photogrammetry for DoDs in deglaciating environments: challenges and opportunities 

Leona Repnik, Arnaud Breillad, Alessandro Giovanardi, Francesco Comiti, Mattia Gianini, Anne-Laure Argentin, Felix Pitscheider, and Stuart N. Lane

Climate change is resulting in rapidly increasing temperatures in the European Alps, rising twice as fast compared to the global average, and leading to unprecedented glacier retreat. Deglaciating alpine landscapes are considered extremely dynamic, evolving rapidly over space and time. The use of DEMs (Digital Elevation Models) of Difference (DoDs) to study changes occurring in these environments has significantly increased in the last years and has been used for a wide range of disciplines. This approach builds on the growing availability of datasets (e.g. historical imagery), accessibility of drones and their sensors (e.g. LiDAR) and facilitated use of digital photogrammetry through commercial and open-source Structure-from-Motion software. However, DoDs of deglaciating landscapes tend to disregard the diversity and complexity of processes in these environments. 

In this research, DEMs were obtained using aerial archival photogrammetry (1977) for the Turtmann basin, a rapidly deglaciating Alpine valley in the Canton of Valais (southwestern Switzerland. A 2021 DEM was used as a reference to create a DoD of the basin (28km2), in order to determine net sediment erosion and deposition during this 44-year time period. 

Most changes identified in the DoD could not be attributed to sediment displacement, but rather to various ecological (e.g. tree growth), glacial (e.g. glacier ice melt) and periglacial (e.g. rock glacier and buried ice melt) processes, as well as error in the photogrammetry. The latter is amplified by the inherently steep topography of alpine basins, which means that small georeferencing errors can cause significant apparent vertical change. A series of post-processing steps were required to obtain precise sediment volumes from the DoD. 

DoDs are extremely valuable for assessing changes in rapidly deglaciating environments. However, challenges exist when applying them to such topographically complex and dynamic landscapes. These challenges must be identified and thoroughly dealt with through DoD post-processing in order to exploit DoDs to their full potential and obtain precise volumes of change. The specific post-processing steps will depend on (1) the research objective, which determines the desired precision as compared to the limits of detection, and (2) the spatial and temporal scales of the DoD, which influence the detectability of changes. In this research, the large temporal (decades) and spatial (basin-wide) scales exposed the challenges and opportunities of using DoDs in rapidly deglaciating environments. The workflow developed to overcome these challenges can be applied to other alpine basins for more precise change detection and thus allow for a better quantitative understanding of processes in deglaciating environments. 

How to cite: Repnik, L., Breillad, A., Giovanardi, A., Comiti, F., Gianini, M., Argentin, A.-L., Pitscheider, F., and Lane, S. N.: Historical photogrammetry for DoDs in deglaciating environments: challenges and opportunities, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6774, https://doi.org/10.5194/egusphere-egu25-6774, 2025.

EGU25-11270 | ECS | PICO | GM2.5

Landscape attractiveness – It depends on the observer 

Magdalena Koschmieder, Christina Pfeuffer, Sebastian Mikolka-Flöry, and Tobias Heckmann

Different people perceive landscapes in various ways depending on their cultural and social background as well as their own values. However, characteristics inherent in the landscapes also have an impact on their perceived beauty. Accordingly, it remains unclear to what extent personal assessments and landscape properties influence how much people appreciate landscapes. In this study, we had 50 test subjects evaluate alpine landscapes represented by 30 historic and recent rendered pictures each. Since the recent pictures should display the exact same part of the landscape as the historic ones, digital elevation models (DEMs) and orthophotos were used to render the current scene in the same greyscale range as in the historic photographs. Additionally, DEMs and landcover maps for the captured images were analysed. These results were used to explain the test subjects’ values of the appreciation of and desire to travel to the landscapes using linear mixed models.

The key finding is that perceived landscape attractiveness depends more on the people assessing the landscapes than the landscape characteristics themselves. The number of distance zones (surrounding, near, middle and far zone) present in the viewshed has a significant impact on the appreciation of the landscape. The maximum slope affects the desire to travel to the landscapes, and the relief energy, the viewshed size and the ratio of the recently glaciated area influence both the appreciation of and the desire to travel to the landscape. Furthermore, the historic photographs are perceived as more beautiful than the recent rendered ones. Taking into account the ratio of the glaciated area, this difference is even more pronounced for the desire to travel to the landscape. The bigger the difference in the glaciated area between the historic and recent image is – hence the more glacier has melted – the more the test subjects desire to travel to the scene shown in the historic picture than in the recent one.

How to cite: Koschmieder, M., Pfeuffer, C., Mikolka-Flöry, S., and Heckmann, T.: Landscape attractiveness – It depends on the observer, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11270, https://doi.org/10.5194/egusphere-egu25-11270, 2025.

EGU25-12156 | ECS | PICO | GM2.5

Deep Learning-based Terrain Data Completion with Geomorphological Constraints 

Tianxin Lu and Michel Jaboyedoff

Raw terrain data acquired by sensing techniques such as SfM or LiDAR typically contain non-terrain components that require filtering, such as vegetation occlusion and other non-terrain features. While filtering helps remove non-terrain data, it can introduce discontinuities and local voids in the dataset. These data gaps can affect both the completeness of the terrain representation and subsequent analysis tasks. Therefore, it is crucial to develop effective terrain data completion methods for reliable terrain analysis.

Traditional terrain data completion methods, such as interpolation-based algorithms and Poisson surface reconstruction, typically model and optimize data continuity from a mathematical perspective. Although these methods address local voids to some extent, they generally fail to exploit terrain features and semantic information, limiting their effectiveness in completing complex terrain scenarios.

To address these issues, we propose a deep learning-based framework for terrain data completion. Our methodology explores different neural network designs with supervised and unsupervised learning, incorporating geomorphological constraints to improve terrain feature representation and semantic understanding. The framework leverages the representational capabilities of deep learning to improve the robustness of terrain data completion, contributing to a more consistent and reliable basis for subsequent terrain analysis and applications.

How to cite: Lu, T. and Jaboyedoff, M.: Deep Learning-based Terrain Data Completion with Geomorphological Constraints, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12156, https://doi.org/10.5194/egusphere-egu25-12156, 2025.

EGU25-15301 | ECS | PICO | GM2.5

Multiple airborne sensors to monitor rafts and beached Sargassum in the Mexican Caribbean: Documenting different UAVs applications for management actions. 

Napoleon Gudino-Elizondo, Eduardo Cuevas, Abigail Uribe-Martinez, Hector Garcia-Nava, Xavier Flores-Vidal, and Orlando Avendaño-Gastelum

The assemblage of multiple sensors on Unmanned Aerial Systems (UAS) to collect high resolution geospatial data represents one of the most significant advances in remote sensing, including oceanographic applications. Coastal inundation of pelagic Sargassum has been thoroughly documented as a natural hazard that jeopardizes the ecological integrity of coastal ecosystems, unbalancing several livelihoods and local economies. Sargassum patches (rafts) are drifted offshore by surface ocean currents, with distinct drivers at different geographic and time scales. UAVs have revolutionized the immediate local remote sensing of Sargassum as they can identify rafts that are expected to reach the coast in terms of hours, becoming a strategic tool for rapidly management actions, bridging the on-site actions with high and medium resolution satellite detections. To obtain primary data on the extent, frequency, and magnitude of floating and beached Sargassum in the Mexican Caribbean, a rapid assessment protocol based on aerial photogrammetric techniques was implemented in the Yucatan Peninsula. We documented the arrival of sargassum rafts in the nearshore environment used to perform statistical comparisons with other remote sensing products. High resolution orthomosaics, DSMs, and 3D reality models were created to document the extent and quantity of beached Sargassum and the contiguous “brown tide” areas. Floating sargassum rafts were also identified in real time using long-range telemetry UAVs between 2 and 20 km offshore, that were consistent with field-based observations. Ocean circulation model outputs are also presented, which demonstrate that including UAV-mounted multi-sensors data acquisition is fundamental towards a comprehensive description and monitoring of the Sargassum coastal dynamics. These results strongly suggest that UAV-derived cartographic products represent an efficient tool for Sargassum-management actions, downscaling satellite detections and linking them with local observations, a strategy that needs to keep addressing as the future research agenda in Operational oceanography.

How to cite: Gudino-Elizondo, N., Cuevas, E., Uribe-Martinez, A., Garcia-Nava, H., Flores-Vidal, X., and Avendaño-Gastelum, O.: Multiple airborne sensors to monitor rafts and beached Sargassum in the Mexican Caribbean: Documenting different UAVs applications for management actions., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15301, https://doi.org/10.5194/egusphere-egu25-15301, 2025.

EGU25-15820 | ECS | PICO | GM2.5

Constraining centennial to sub-annual sediment dynamics on alpine alluvial fans – first insights from the Friedergries (Germany) 

Philipp Gewalt, Thomas C. Wagner, and Michael Krautblatter

Alpine alluvial fans are important storages in the alpine sediment cascade. It is to be expected that climate change and the resulting changes in precipitation will have a massive impact on the dynamics of alpine alluvial fans. In order to differentiate between short-term and long-term dynamics, we compile a dataset quantifying sediment redistribution of a small mountain river and its alluvial fan on centennial, decadal and sub-annual scales. Our dataset comprises historical topographic maps from 1826 to 1912, 25 sets of historical aerial images collected between 1945 and 2024, and 17 high-resolution UAV-campaigns collected between September 2018 and October 2024. We identify the spatial changes in the sediment body, quantify the sediment redistribution and relate both to precipitation.

On centennial timescales, our data show a shift from presumably low geomorphic activity that persisted for at least 100 years (1820s-1930s) in the eastern sector of the fan, to high geomorphic activity with rapid channel migration across the central fan within the past 60 years. The onset of intense geomorphic activity may be contemporaneous to the increase in debris flow activity at nearby lake Plansee in the 1920s (Kiefer, Oswald et al., 2021). Decadal changes to the active area are largely explained by median precipitation (r2 = 0.66, p < 0.002) measured at a weather station c. 10 km east. Since the 1960s, incision at the apex and deposition at the toe of the fan can be observed. Sub-annual change detections show that for most epochs, erosion and deposition balance out within the uncertainty margin and the main channel gradually shifts its position by bank erosion and gravel bar construction. However, following an extreme deposition event between August and September 2019 with a net deposition of 8000 ± 3500 m3, the course of the main channel abruptly shifted. Our preliminary results show that while historical maps and aerial images are useful to reconstruct long-term trends, repeat topographic surveys with a close temporal spacing are needed to understand the processes behind these trends.

Kewords: alpine alluvial fan, sediment redistribution, geomorphic change detection, multiscale investigation

Kiefer, C., Oswald, P. Moernaut, J., Fabbri, S.C., Mayr, C., Strasser, M. & Krautblatter, M. (2021): A 4000-year debris flow record based on amphibious investigations of fan delta activity in Plansee (Austria, Eastern Alps). – Earth Surface Dynamics, 9: 1481–1503. DOI: 10.5194/esurf-9-1481-2021

How to cite: Gewalt, P., Wagner, T. C., and Krautblatter, M.: Constraining centennial to sub-annual sediment dynamics on alpine alluvial fans – first insights from the Friedergries (Germany), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15820, https://doi.org/10.5194/egusphere-egu25-15820, 2025.

EGU25-16381 | PICO | GM2.5 | Highlight

A new high resolution historical aerial image dataset from East Greenland 

Anders Bjork, Anna Deichmann, and Tobias Socher

During the last decades the high Arctic has undergone substantial changes as a result of global warming and arctic amplification. Melt seasons are expanding rapidly, and landscape and ecosystems are shifting into new states. To quantify these changes from the historical baseline requires datasets on pre-warming states, which can be extremely rare in the high Arctic. Prior to the satellite era, starting in the 1990s, a commonly used data source for baselines in geosciences is aerial photographs, which if one is lucky can reach back to the 1930s. These aerial images are most often recorded at high elevation and perhaps also obliquely which results in spatial resolutions of 2-10 meters, limiting the level of detail that can be resolved on the ground.  

With this presentation we reveal a new exciting dataset of aerial images from East Greenland recorded in the 1950s and ‘60s. Contrary to other aerial campaigns, these images were recorded at very low elevation in order to conduct geological mapping, ultimately yielding spatial resolutions surpassing those of the newest high resolution satellites.

The images were recorded by geologist John Haller during the Lauge Koch expeditions to central East Greenland in the 1950s and 1960s, and comprise a dataset of c. 3600 high resolution oblique images recorded at low elevation from plane and helicopter. The images are recorded in stereo, which allows us to recreate the terrain surface in 3D and construct orthorectified imagery that allows a direct comparison with modern satellite images, for use in all aspects of landscape- and ecosystem evolution.

How to cite: Bjork, A., Deichmann, A., and Socher, T.: A new high resolution historical aerial image dataset from East Greenland, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16381, https://doi.org/10.5194/egusphere-egu25-16381, 2025.

EGU25-17688 | ECS | PICO | GM2.5

Advances in Historical Aerial Image Analysis: Boosting SfM Pipelines with Learned Models 

Lucas Kugler, Francesco Ioli, Jan Dirk Wegner, Inés Dussaillant, Camilo Rada, and Livia Piermattei

Trend determination for earth surface processes requires long and continuous and certain measurements, but long-term records of landscape change are often limited in temporal and spatial extent. Scanned historical aerial imagery serve as a valuable resource to derive data products like digital elevation models (DEMs) to document the historical state of the Earth's surface and to calculate trends for different processes e.g. glacier dynamics.

Classic Structure-from-Motion (SfM) photogrammetry workflows have demonstrated the capability to automatically generate DEMs and orthoimage mosaics from such historical images, as highlighted in a few studies. These workflows typically consist of the following steps: (a) pre-processing, (b) tie-point extraction, (c) matching, (d) bundle adjustment, (e) dense reconstruction, (f) co-registration, and (g) orthoimage mosaic generation. However, classic methods struggle with the challenges historical imagery coming with. For example: inconsistent image quality, limited metadata documentation, image distortions and distinct viewpoint geometries.

Recently, advances in robotics and computer vision have introduced learned models for tasks such as tie-point identification, matching, dense reconstruction as well as part of the co-registration stage (e.g. SuperPoint, ALIKE, SuperGlue, LoFTR and more). These networks have shown promising results in different stereo-matching scenarios by outperforming classic SfM methods. However, since they were primarily developed for modern robotics and computer vision tasks, their performance on scanned historical aerial imagery remains uncertain. As historical imagery exhibits the properties described above, these networks were not optimised with them during training.

We boost existing pipelines in tie-point extraction and matching with these models and compare the quality of resulting DEMs from different model combinations together. We also highlight issues encountered when applying these learned models to historical aerial imagery and proposes solutions to address them. We demonstrate our findings using scanned historical images from the Southern Patagonian Ice Field (Chile) recorded in 1980, particularly for the Grey & Dickson Glacier area, as well the south-west flank of Cordon Mariano Moreno Mountain and adjacent fjords. These two sites providing different acquisition geometries and overlaps. The results evaluate the average RMS reprojection error following the bundle adjustment, to determine the quality of different extractors and matchers as well as the median distance between closest points to evaluate the co-registration.

How to cite: Kugler, L., Ioli, F., Wegner, J. D., Dussaillant, I., Rada, C., and Piermattei, L.: Advances in Historical Aerial Image Analysis: Boosting SfM Pipelines with Learned Models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17688, https://doi.org/10.5194/egusphere-egu25-17688, 2025.

Along many coastlines worldwide, a variety of direct and indirect anthropogenic influences are influencing natural processes of coastal erosion and deposition.  Both traditional change reconstruction and monitoring techniques (e.g. repeat surveys) and increasingly sophisticated approaches (e.g. photogrammetry, LiDAR, drone imagery) require specialist knowledge and equipment, can be time consuming to apply, and may be restricted to assessing relatively recent changes over short timeframes (e.g. typically years to a few decades).  Here, we evaluate the potential for archival visual sources - maps, paintings, geological sketches, and historical photographs – to help document changes in the coastal environment of Ceredigion County, west Wales, over the past 100-150 years.  Two extant sites of geoscientist interest, both located within 20 km of Aberystwyth, were investigated: Harp Rock (Craig y Delyn), which represents the westward-dipping limb of a synclinal fold, and Monk’s Cave (Twll Twrw), which has essentially now developed into a coastal arch.  Egg Rock (Tŵr Gweno), a coastal stack which was previously located near to Monk’s Cave but has since disappeared, was also investigated.  All three sites were well-known tourist attractions in the late 1800s and early 1900s, and various maps, paintings, sketches and photographs help to provide both qualitative and quantifiable insights into the nature of coastal change, including the sequencing, rates, and timing of key changes, as well as volumes of mass loss.  For example, Harp Rock is retreating landward as sandstone strata of ~37 cm thickness are removed by wave action and mass movement; for every 1 m2 of stratal loss, a mass of 858.4 kg is removed.  For Monk’s Cave, the average vertical erosion rate of the cave entrance is estimated to ~0.65 cm/yr over a timespan of 139 years.  Based on the last known photograph of Egg Rock (early 1900s), the total mass loss is approximated to be 197.70 t.  Collectively, the findings from these three sites provide insights into rates of Holocene shore platform development along this dynamic coastline.

Wider use of archival visual sources clearly has potential for complementing more technically sophisticated short-term change reconstruction and monitoring approaches.  Key challenges include sourcing well-dated, high-quality archival visual sources to enable establishment of robust timelines of change and the generation of quantitative data, and safely accessing potentially hazardous locations to enable new paintings, sketches, or photography.  If these challenges are surmounted, opportunities include enhanced potential for: i) providing quantified landscape change case studies for inclusion in school/university geoscience syllabi; ii) demonstrating the relevance of geoscience for local/regional natural and cultural heritage; and iii) enhancing public engagement with coastal geoscience (e.g. through citizen science projects or science-art collaborations).

 

How to cite: Goode, C. and Tooth, S.: Can archival visual sources be used to quantify coastal change?: insights from the dynamic coastline of Ceredigion, west Wales, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18399, https://doi.org/10.5194/egusphere-egu25-18399, 2025.

EGU25-124 | Posters on site | PS1.1

Solar wind- Mercury's magnetosphere interaction by data exploration and MHD simulations 

Shu-Hua Lai, Yung-Ching Wang, Ya-Hui Yang, and Wing-Huen Ip

Mercury's magnetosphere is more dynamic than Earth's due to its proximity to the Sun, and it is subject to a lower Mach number solar wind. Regarding the solar wind interaction with Mercury, we are interested in the configurations of Mercury’s magnetosphere and the energy transport under various solar wind conditions. First, this study examines the potential impact of low Mach number solar wind on Mercury's bow shock and the resulting effects on the magnetosphere. To analyze the variability of Mercury's bow shock in response to solar wind properties, this study combines observations by the Helios data with theoretical solutions and MHD simulations. The results show that when Mercury encounters solar wind with an extremely low Mach number, its bow shock is expected to become more flattened, further from the planet, and may even disappear completely. Our other focus is on the Kelvin-Helmholtz instability (KHI) that occurs at the magnetopause, which plays a crucial role in the energy transfer and momentum coupling process between the solar wind and Mercury's magnetospheres. We conducted MHD simulations based on boundary conditions and plasma parameters from a global hybrid simulation of the MESSENGER’s first flyby in 2008. Given the lack of comprehensive plasma observations of Mercury's magnetosphere, we examined two scenarios: one with a heavily mass-loaded magnetosphere and another with a weakly mass-loaded magnetosphere. Our findings show that the KHI in a heavily loaded magnetosphere results in a more turbulent magnetopause, with nonlinear fast-mode plane waves expanding away from the magnetopause. The momentum and energy flux quantified from our simulations reveals that the KHI with a heavily loaded magnetosphere can efficiently transport momentum and energy away from the magnetopause in the presence of the fast-mode plane waves. In such a scenario, observed in the inner magnetosphere, the momentum flux can reach about 0.5 % of the initial solar-wind dynamic pressure; the energy flux can be 10-2 erg/cm2/s, and the energy density is about 1.5 %-3.0 % of the initial solar-wind energy.

How to cite: Lai, S.-H., Wang, Y.-C., Yang, Y.-H., and Ip, W.-H.: Solar wind- Mercury's magnetosphere interaction by data exploration and MHD simulations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-124, https://doi.org/10.5194/egusphere-egu25-124, 2025.

EGU25-1275 | Orals | PS1.1

Investigation of the Ultralow Frequency (ULF) foreshock boundary at Mercury 

Tomas Karlsson, Xóchitl Blanco-Cano, Heli Hietala, Sofia Bergman, Ferdinand Plaschke, and Tsz Kiu Wong Chan

Ultralow frequency (ULF) waves are found in certain parts of the upstream region of planetary bow shocks. These waves are believed to be driven by the interaction of solar wind ions reflected from the bow shock with the original solar wind beam. The region where ULF waves can possibly be observed is then determined by the regions accessible to the reflected ions within the foreshock (defined as the region magnetically connected to the bow shock). The boundary of the region where ULF waves are observed at Earth is known to also depend on the growth rate of the waves and on the direction of the interplanetary magnetic field (IMF). To identify the ULF foreshock boundary at Mercury, we use MESSENGER observations to investigate the presence or absence of clear ULF wave activity upstream of the bow shock. The boundary of regions where ULF waves are present, as parametrized by the angle θBn between the IMF and the bow shock normal, is identified and the dependence on the IMF is studied. The connection to higher-frequency whistler waves emissions is also investigated. The results are compared to results from other planets, and their connection to other upstream phenomena is discussed. Finally, open questions that can be addressed by the upcoming BepiColombo mission are discussed.

How to cite: Karlsson, T., Blanco-Cano, X., Hietala, H., Bergman, S., Plaschke, F., and Wong Chan, T. K.: Investigation of the Ultralow Frequency (ULF) foreshock boundary at Mercury, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1275, https://doi.org/10.5194/egusphere-egu25-1275, 2025.

EGU25-2481 | Posters on site | PS1.1

Mercury upstream region as a natural laboratory of beam plasma experiments 

Yasuhito Narita, Daniel Schmid, and Uwe Motschmann

Upstream region of the Mercury magnetosphere is of great interest in advancing our knowledge on the plasma waves and instabilities. The interplanetary magnetic field is nearly aligned with the solar wind stream at the distances of Mercury to the Sun with a Parker spiral angle of only about 20 degrees. A one-dimensional beam plasma system is likely realized ahead of or around the Mercury. The solar wind plasma streams away from the Sun and the beam ions (either shock-reflected ions or pickup ions) stream against the sola wind, forming a naturaly laboratory of head-on beam collider experiments at an energy scale of keV (through the electromagnetic interactions without binary collisions). We study the dielectric response of the beam plasma and develop various scenarios of beam instabilities relevant to the Mercury upstream waves in a systematic way including the right-hand resonant instability and the pickup ion cyclotron waves. Our wave model has the potential to serve as an analysis tool to estimate the beam velocity and the flow speed from the resonance frequency, particularly useful to in-situ magnetic field data analyses for MESSENGER and BepiColombo measurements.

How to cite: Narita, Y., Schmid, D., and Motschmann, U.: Mercury upstream region as a natural laboratory of beam plasma experiments, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2481, https://doi.org/10.5194/egusphere-egu25-2481, 2025.

EGU25-3409 | ECS | Posters on site | PS1.1

A Survey of the Anomalous Reconnection Layer on Mercury 

I-Hsiang Chiu, Jih-Hong Shue, Hiroshi Hasegawa, Jun Zhong, and Masafumi Hirahara

Abstract

Anomalous reconnection layer (ARL) usually appears near the magnetopause when the solar wind is in low Alfvén Mach number. The structure of an ARL is similar to the magnetic reconnection outflow region, i.e., a decrease in the total magnetic field and an increase in the high-energy ion flux. The ARL is seldom observed in the Earth’s magnetospheric environment because the solar wind at Earth is mostly in high Alfvén Mach number regime. According to previous observations, the solar wind at Mercury is usually in low Alfvén Mach number. Therefore, we assume that such an ARL can be observed frequently near Mercury’s magnetopause. To test this assumption, we examined the magnetic fields and ion fluxes obtained at the Mercury’s magnetosheath by the MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft. With 120 events of ARLs we identified from MESSENGER’s data, we validate the assumption that ARLs frequently appear on Mercury. These ARL events were extracted from the list of MESSENGER bowshock and magnetopause crossing times compiled by Winslow et al. [2013]. The number of the ARL events found on Mercury is much larger than those found on Earth. The thickness of each ARL was estimated from the data, finding that the ARLs occupy, on average, one-fifth the thickness of the magnetosheath for Mercury. This work helps deepen our understanding of the comparative magnetospheric environment of Mercury and Earth.

 

References

Winslow, R. M., B. J. Anderson, C. L. Johnson, J. A. Slavin, H. Korth, M. E. Purucker, D. N. Baker, and S. C. Solomon (2013), Mercury's magnetopause and bow shock from MESSENGER Magnetometer observations, J. Geophys. Res. Space Physics, 118, 2213–2227, doi:10.1002/jgra.50237.

How to cite: Chiu, I.-H., Shue, J.-H., Hasegawa, H., Zhong, J., and Hirahara, M.: A Survey of the Anomalous Reconnection Layer on Mercury, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3409, https://doi.org/10.5194/egusphere-egu25-3409, 2025.

EGU25-3985 | ECS | Posters on site | PS1.1

 Impact Vaporization and Mercury’s Superthermal Exosphere 

Ian-Lin Lai, Chen-Yen Hsu, and Wing-Huen Ip

Mercury’s tenuous atmosphere leaves its surface exposed to continuous meteoroid bombardment, which vaporizes surface material and enriches the exosphere with various species. Ground-based observations (Bida et al., 2000; Killen et al., 2005) first detected calcium in Mercury’s exosphere; subsequent measurements by the MASCS spectrometer onboard MESSENGER confirmed that these Ca atoms can reach remarkably high temperatures (12,000–20,000 K, and occasionally up to ~70,000 K) despite Mercury’s surface being only a few hundred K (Killen et al., 2005). The Ca corona also displays distinct temporal and spatial patterns, suggesting that meteoroid impact vaporization—especially from the 2P/Encke meteor stream—is a significant source of these superthermal Ca atoms. It has been proposed that Ca-bearing molecules, such as CaO, are vaporized by impacts and subsequently dissociated into Ca atoms. In this work, we employ a time-dependent Monte Carlo model to simulate the expansion of gases released by impact vaporization, incorporating multiple species and photodissociation processes to determine the spatial distribution of fragments. These results will aid in interpreting future observations by the BepiColombo mission.

How to cite: Lai, I.-L., Hsu, C.-Y., and Ip, W.-H.:  Impact Vaporization and Mercury’s Superthermal Exosphere, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3985, https://doi.org/10.5194/egusphere-egu25-3985, 2025.

EGU25-4305 | ECS | Posters on site | PS1.1

Roughness map for the equatorial region of Mercury and its implication to surface evolution 

Gaku Nishiyama, Frank Preusker, Adrien Broquet, Alexander Stark, and Hauke Hussmann

Analyses of topographic roughness at various baselines are useful for studying surface evolution on airless bodies. Using data from the Mercury Laser Altimeter (MLA) onboard Space ENvironment, Geochemistry, and Ranging (MESSENGER) mission, roughness distribution on Mercury has been investigated at baselines down to sub-km scale [e.g., 1]. However, due to the eccentric orbit of MESSENGER and the limited ranging distance of MLA, laser ranging observations are limited to the north polar region. In addition, previous image-based digital elevation cannot be used to quantify roughness at km scale due to limited spatial resolution [2]. Therefore, roughness at km-scale baselines has not been mapped below 45°N latitude on Mercury.

To complement the lack of roughness data in the equatorial region, this study analyzes the latest global DEM (version 20240927) produced as described in Preusker et al. [3]. The effective resolution of this DEM has been estimated to be 5 km [e.g., 3]. Focusing on topographic curvatures at baselines of 5–10 km and their interquartile ranges at each latitude and longitude, we mapped roughness distribution at latitudes of 66°N–66°S to examine correlations between roughness and geologic features.

Our new roughness map shows several anomalous features correlated with Mercury’s geology. The most obvious feature is a clear distinction between smooth plains and rough intercrater plains. Our roughness map shows roughness differences similar to those reported by previous works for the northern hemisphere [1]. In addition, our analysis shows a certain variation in roughness among the smooth plains. For example, the Caloris smooth plains show higher roughness than other smooth plains due to superposing grabens in the Caloris basin. Another characteristic is high-roughness anomalies around young basins. The areas of continuous ejecta have higher roughness than the surroundings due to their freshness. The roughness values do not simply decrease with increasing distance from the basin centers but show local minima adjacent to their rims, originating from coverage of impact melt and/or deficit of secondary craters.

Furthermore, a comparison with the latest catalog of tectonic landforms [4] shows an absence of contractional landforms at high roughness anomalies. The lobate scarps and ridges tend to be distributed outside rough regions like the young basin ejecta. This correlation may suggest superposition of younger basin ejecta on older tectonic features, difficulty of tectonic landform detection on rough terrains, and/or less efficient formation of contractional landforms due to possibly high crustal porosity. These possibilities imply that the extent of Mercury’s radial contraction may have been underestimated due to the obscuration of old contractional landforms. In the presentation, we will discuss possible extent of corrections to global contraction estimates to account for the roughness effect.

References:

[1] Kreslavsky M. A. et al. (2014) GRL, 41, 8245–8251.

[2] Florinsky I. V. (2018) Planetary and Space Science, 151, 56–70.

[3] Preusker F. et al. (2017) Planetary and Space Science, 142, 26–37.

[4] Klimczak C. et al. (2023) 54th LPSC, Abstract #1122.

Acknowledgment: This work was supported by JSPS KAKENHI Grant Number JP22K21344 and JSPS Overseas Research Fellowship.

How to cite: Nishiyama, G., Preusker, F., Broquet, A., Stark, A., and Hussmann, H.: Roughness map for the equatorial region of Mercury and its implication to surface evolution, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4305, https://doi.org/10.5194/egusphere-egu25-4305, 2025.

EGU25-6716 | Posters on site | PS1.1

Insights into Mercury's Hydrogen Exosphere: Characterization and First Detection of H₂ Molecules 

Fabian Weichbold, Daniel Schmid, Helmut Lammer, Martin Volwerk, Manuel Scherf, Nikolai Erkaev, Ali Varsani, and Cyril Simon-Wedlund

Between 1974 and 1975, the Mariner 10 spacecraft investigated Mercury's environment during three flybys. By using its ultraviolet spectrometer, it identified helium, atomic oxygen, and hydrogen atoms in Mercury’s exosphere. Interestingly, no H2 molecules were detected during these flybys. Based on data from the occultation instrument, an upper limit for H2 surface density was established from the detection threshold of about 1.4 x 107 cm-3. Here, we present the first in-situ detection of H2 molecules in the Hermean Exosphere, identified through magnetic field and plasma measurements obtained from the MESSENGER spacecraft. The data was analyzed for ion cyclotron waves produced by H2+ pick-up ions. Our findings reveal a much lower dayside surface density of approximately 2000 cm-3, significantly below the Mariner 10 detection threshold. Furthermore, the observed atomic hydrogen in the exosphere cannot be entirely attributed to H2 dissociation. Instead, it likely arises from a combination of thermal hydrogen atoms, charge exchange processes, space weather effects, H2 dissociation and micrometeorite impacts.

How to cite: Weichbold, F., Schmid, D., Lammer, H., Volwerk, M., Scherf, M., Erkaev, N., Varsani, A., and Simon-Wedlund, C.: Insights into Mercury's Hydrogen Exosphere: Characterization and First Detection of H₂ Molecules, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6716, https://doi.org/10.5194/egusphere-egu25-6716, 2025.

EGU25-6945 | Orals | PS1.1

Observations from the Mercury Electron Analyzer onboard BepiColombo during its sixth Mercury flyby 

Nicolas André, Jean-André Sauvaud, Yoshifumi Saito, Mathias Rojo, Sae Aizawa, Andrei Fedorov, Emmanuel Penou, Alain Barthe, Shoichiro Yokota, Zdenek Nemecek, Jana Safrankova, Maria Federica Marcucci, Zhi-Yang Liu, Moa Persson, Lina Hadid, Dominique Delcourt, Yuki Harada, Markus Fraenz, Norbert Krupp, and Go Murakami

On 8 January 2025, the ESA/JAXA BepiColombo mission flew by Mercury for the sixth time at an altitude of 295 km. The spacecraft took on a unique route through Mercury’s magnetic and particle environment, crossing the equator opposite the Sun on Mercury’s night side before flying over the planet’s north pole. During eclipse, in the cold shadow of the planet, as well as above the northern pole the spacecraft passed through regions where charged particles precipitate from the planet’s magnetic tail and from the solar wind towards its surface. We will detail the original electron observations obtained by the Mercury Electron Analyzer during Mercury’s sixth flyby, and compare and contrast them with electron observations obtained during previous BepiColombo flybys. All together, these new observations will provide new insights into the diversity of structures observed in these regions and the underlying mechanisms responsible for their formation and dynamics.

 

How to cite: André, N., Sauvaud, J.-A., Saito, Y., Rojo, M., Aizawa, S., Fedorov, A., Penou, E., Barthe, A., Yokota, S., Nemecek, Z., Safrankova, J., Marcucci, M. F., Liu, Z.-Y., Persson, M., Hadid, L., Delcourt, D., Harada, Y., Fraenz, M., Krupp, N., and Murakami, G.: Observations from the Mercury Electron Analyzer onboard BepiColombo during its sixth Mercury flyby, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6945, https://doi.org/10.5194/egusphere-egu25-6945, 2025.

EGU25-6978 | ECS | Posters on site | PS1.1

Mercury's Nightside Magnetosphere: Predictions for Mercury's Magnetotail Twist at the Orbits of MPO and Mio 

Willi Exner and Norberto Romanelli

Planetary magnetospheres exhibit significant twisting of the magnetotail with increasing downstream distances.
However, Mercury's tail twist observed by MESSENGER indicate a rather small twist of up to 3 degrees.
Here, we model Mercury's magnetotail response to different Interplanetary Magnetic Field (IMF) directions and determine what MPO and Mio might observe in their orbital phase with the hybrid model AIKEF.
Our hybrid model results indicate that Mercury's magnetotail topology exhibits a similar small twist at MPO altitudes, comparable to MESSENGER results.
The tail twist observed by Mio, however, indicates a strong dependency on the upstream IMF direction, becoming much more Earth-like.
In addition, kinetic effects warp and bend the neutral sheet significantly, disallowing easy determinations of the twist angles.

How to cite: Exner, W. and Romanelli, N.: Mercury's Nightside Magnetosphere: Predictions for Mercury's Magnetotail Twist at the Orbits of MPO and Mio, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6978, https://doi.org/10.5194/egusphere-egu25-6978, 2025.

Mercury, the innermost planet in our solar system, offers a unique natural laboratory for planetary science, particularly with its unexpectedly high concentration of volatile elements and the presence of volatile-related geological features. This study investigates the morphology and ages of craters at Mercury's north and south poles to understand the distribution of water ice within these regions. Utilizing high-resolution images from the MESSENGER mission and various digital elevation models, we measured crater depth and diameter and conducted crater size-frequency distribution analyses. Our findings reveal significant differences in the depth-to-diameter (d/D) ratios and absolute ages of craters between the poles. North Pole craters are generally younger, deeper, and smaller in diameter, while South Pole craters are older, shallower, and larger in diameter. The Northern Smooth Plains at the North Pole, formed by extensive volcanic activity, exhibit fewer impact craters, suggesting a younger surface. In contrast, the South Pole's heavily cratered terrain displays significant weathering and thicker regolith layers. The study also highlights the uneven distribution of water ice, likely influenced by crater morphology and the presence of insulating layers. This research provides insights into the geological history of Mercury and the processes shaping its polar regions, enhancing our understanding of the planet's volatile content and its implications for habitability in the inner solar system.

How to cite: Wang, X.: Asymmetry distribution of craters on north and south poles of Mercury, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7516, https://doi.org/10.5194/egusphere-egu25-7516, 2025.

EGU25-7859 | ECS | Posters on site | PS1.1

Kelvin-Helmholtz Instability Observations on Mercury’s magnetopause: MESSENGER Study 

Ruotan Li, Weijie Sun, and Suiyan Fu

Kelvin-Helmholtz (K-H) instability plays an important role in transporting mass, momentum and energy at the magnetopause of planetary magnetospheres. Previous studies have shown that the K-H waves on Mercury’s magnetosphere exhibit clear dawn-dusk asymmetry, i.e., they are frequently observed on the duskside magnetopause but rarely on the dawnside. In this presentation, we first present a case study of K-H waves on the dawnside of Mercury’s magnetosphere and a  statistical study of K-H waves from 2014 to 2015 based on MSEEENGER’s observations.

In the case study, the K-H waveforms on the dawnside side were divided into linear waves and nonlinear waves by modeling the magnetopause as Harris current sheet. The 30mHz compressional ultra-low-frequency waves and ion-Bernstein modes were observed in the magnetosphere adjacent to these K-H waves, which are interpreted as the evidence of energy and mass transport by K-H waves. However, only a few magnetopause oscillations were observed on the duskside during the same MESSENGER’s orbit under similar interplanetary magnetic field conditions. No compressional waves or ion-Berstein modes were observed associated with these oscillations. 

Our statistical study found that K-H waves were equably prevalent on both the dawnside and duskside, which are different from the previously reported dawn-dusk asymmetry. We categorized our cases into linear and nonlinear stages and analyzed their interplanetary magnetic field conditions. Our results provide  insights into the study of K-H instability at Mercury, especially the mechanism of asymmetry and transport of plasma and energy.

How to cite: Li, R., Sun, W., and Fu, S.: Kelvin-Helmholtz Instability Observations on Mercury’s magnetopause: MESSENGER Study, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7859, https://doi.org/10.5194/egusphere-egu25-7859, 2025.

EGU25-8218 | Orals | PS1.1

Extreme Space Weather at Mercury: Investigating Magnetospheric and Surface Interactions Using Hybrid Simulations 

Shahab Fatemi, Paul S. Szabo, Andrew R. Poppe, Jim M. Raines, and Anna Millilo

Mercury’s intrinsic magnetic field is remarkably weak, resulting in a small magnetosphere. Due to the proximity of Mercury to the Sun and lack of a protective ionosphere, Mercury’s magnetosphere endures the most intense solar wind flux and severe space weather in the solar system. The interaction between the solar wind and Mercury’s magnetosphere is dominated by dynamic kinetic processes, such as exceptionally high magnetic reconnection rates. Mercury’s magnetosphere is also closely coupled to its surface, making it highly susceptible to extreme solar events, including Coronal Mass Ejections (CMEs). To explore this complex and dynamic environment, we utilize Amitis (https://www.amitiscode.com), an advanced 3D hybrid-kinetic plasma model, to simulate the interaction between the solar wind and Mercury’s magnetosphere under conditions of extreme solar activity. Our study reveals how Mercury’s magnetosphere dynamically responds to intense solar events and provides detailed insights into the energy and flux of solar wind plasma impacting the planet’s surface. By examining these interactions, we aim to better understand the mechanisms governing Mercury’s unique space weather environment and their implications for surface processes.

How to cite: Fatemi, S., Szabo, P. S., Poppe, A. R., Raines, J. M., and Millilo, A.: Extreme Space Weather at Mercury: Investigating Magnetospheric and Surface Interactions Using Hybrid Simulations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8218, https://doi.org/10.5194/egusphere-egu25-8218, 2025.

EGU25-8261 | Posters on site | PS1.1

High resolution geomorphological analysis of Agwo facula (Mercury) 

Lorenza Giacomini, Anna Galiano, Valentina Galluzzi, Giovanni Munaretto, David A. Rothery, Deborah Domingue, John Weirich, Lauren M. Jozwiak, Mario D' Amore, and Cristian Carli

On Mercury, faculae are high-albedo, spectrally red, deposits originating from explosive volcanic eruptions (Kerber et al., 2009) whose source are likely rimless depressions. These depressions are usually located in the center of the facula and interpreted to be volcanic vents. In this work we analyzed the Agwo facula, sited in the western margin of Caloris basin (22.39°N, 146.16°E). We performed a detailed geomorphological map of the area using MDIS derived mosaics with a spatial resolution ranging from 20 m/pixel to 28 m/pixel and with different illumination conditions. Additionally, a BDR (Basemap reduced Data Record) MDIS mosaic, with a resolution of 166 m/pixel, was used as a basemap. MDIS WAC color maps, based on the reflectance at 750 nm and the VIS slope between 480 and 830 nm, respectively, were also used as part of the analysis. These latter maps helped determine the areal extent of the pyroclastic deposits. Finally, a DTM of the region, derived from MDIS images using the technique of stereophotoclinometry (SPC) and with a spatial resolution of 20 m/pixel, helped us to better characterized the facula’s topography. The geomorphological map highlights that Agwo facula experienced several explosive episodes. In particular, through the cross-cutting relationship observed among the pits, at least eight eruptive events have been distinguished. The terrain within the pits shows different surface texture and albedo, that allowed the distinction of several geological units: from the oldest and smoother surfaces to the younger and rougher textured surfaces. Therefore, the morphological and spectral characteristics of pits suggest that Agwo facula is the result of multiple eruptions, which likely occurred at different times, contributing to the better understanding of the formation of this feature.

 

References:

Kerber, L., Head, J.W., Solomon, S.C., Murchie, S.L., Blewett, D.T., Wilson, L., 2009. Earth Planet. Sci. Lett. 285, 263–271. https://doi.org/10.1016/j.epsl.2009.04.037.

 

Acknowledgment

This research was supported by the International Space Science Institute (ISSI) in Bern, through ISSI International Team project #552 (Wide-ranging characterization of explosive volcanism on Mercury: origin, properties, and modifications of pyroclastic deposits). Contributions by D. Domingue and J. Weirich were also supported by NASA’s Solar System Working’s grant 80NSSC21K0165.

How to cite: Giacomini, L., Galiano, A., Galluzzi, V., Munaretto, G., Rothery, D. A., Domingue, D., Weirich, J., Jozwiak, L. M., D' Amore, M., and Carli, C.: High resolution geomorphological analysis of Agwo facula (Mercury), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8261, https://doi.org/10.5194/egusphere-egu25-8261, 2025.

EGU25-8338 | Orals | PS1.1

Observations of Mercury’s plasma environment along BepiColombo’s sixth swingby on 8 Jan 2025 

Norbert Krupp, Markus Fränz, Daniel Teubenbacher, Willi Exner, Daniel Heyner, Lina Z. Hadid, Ali Varsani, Yuki Harada, Sae Aizawa, Nicolas Andre, Anna Milillo, Yoshifumi Saito, Dominique Delcourt, Fabio Prencipe, Harald Krüger, Gunter Laky, Bruno Katra, Christophe Verdeil, Shoichiro Yokota, and Björn Fiethe

The BepiColombo mission to Mercury consists of two spacecraft MPO and MIO and was launched in 2018. During the cruise phase towards the target the spacecraft performed its last close flyby near Mercury on 8 Jan 2025 (MSB6). This was the last flyby before going into orbit around the innermost planet at the end of 2026. We report on particle results from the Mass Spectrum Analyzer MSA on MIO and the Planetary Ion Camera PICAM onboard MPO together with magnetic field data MAG and hybrid simulation during this flyby. PICAM measured solar wind upstream and recorded the magnetospheric and magnetosheath plasma at various energies while MSA recorded the ion composition during the flyby including H+, He++, He+, Na+ and other heavy ions. Most of Na+ was seen near closest approach in the shadow of the planet which agrees well with AIKEF hybrid model results.

 

How to cite: Krupp, N., Fränz, M., Teubenbacher, D., Exner, W., Heyner, D., Hadid, L. Z., Varsani, A., Harada, Y., Aizawa, S., Andre, N., Milillo, A., Saito, Y., Delcourt, D., Prencipe, F., Krüger, H., Laky, G., Katra, B., Verdeil, C., Yokota, S., and Fiethe, B.: Observations of Mercury’s plasma environment along BepiColombo’s sixth swingby on 8 Jan 2025, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8338, https://doi.org/10.5194/egusphere-egu25-8338, 2025.

EGU25-9676 | ECS | Orals | PS1.1

Three-dimensional Global Hybrid Simulation of Magnetosheath Jets at Mercury  

Jin Guo, San Lu, Quanming Lu, James Slavin, Weijie Sun, and Jun Zhong

Plasma high-speed jets are common in Earths magnetosheath, and they significantly perturb the magnetosheath and affect the magnetosphere. The space environment of Mercury, characterized by the bow shock, magnetosheath, and magnetosphere, shares many similarities with that of Earth, so high-speed jets may also be formed in Mercurys magnetosheath. Here we examine the formation of magnetosheath jets using a three-dimensional global hybrid simulation. The simulation results demonstrate that magnetosheath jets may be formed by the passage of upstream compressive structures through the bow shock. The number and size of the jets are significantly smaller than those at Earth because of Mercurys smaller magnetosphere size. Under the impact of magnetosheath jets, Mercurys magnetopause undergoes significant deformation up to 0.19 RM(RMis Mercurys radius). These simulation results are expected to be tested by the BepiColombo mission. 

How to cite: Guo, J., Lu, S., Lu, Q., Slavin, J., Sun, W., and Zhong, J.: Three-dimensional Global Hybrid Simulation of Magnetosheath Jets at Mercury , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9676, https://doi.org/10.5194/egusphere-egu25-9676, 2025.

EGU25-10436 | Posters on site | PS1.1

Mercury’s Environment Observed by BepiColombo during the Second Mercury’s Swing-by 

Anna Milillo, Ali Varsani, Daniel Heyner, Lina, Z. Hadid, Wolfgang Baumjohann, Stas Barabash, and Nicolas Andrè and the MPO/SERENA, MPO-MAG, Mio-MGF, Mio/MPPE-MEA and MSA teams

Thanks to MESSENGER observations, we know that Mercury’s magnetosphere is highly dynamic, and it can be fully reconfigured in a few minutes, with strong influences of external conditions.

BepiColombo mission includes a comprehensive payload for the investigation of the environment. During the cruise phase, not all the sensors can operate for science measurements, however, during the swing-bys the magnetic field and particles in Mercury’s magnetosphere are successfully measured by the MPO and Mio payloads. In this presentation, we will focus on Mercury’s swing-by 2 (MSB2) observations in comparison with other swing-bys. During the MSB2, BepiColombo passed from dusk in the tail toward dawn in the dayside in a nearly equatorial path. The IMF turned from northward to southward during the crossing. The dayside magnetopause boundary was clearly observed, while the bow shock crossing was not clearly distinguishable. Close to the planet signatures of circulating high energy ions have been seen. While upstream the bow shock, foreshock ions have been observed.

How to cite: Milillo, A., Varsani, A., Heyner, D., Hadid, L. Z., Baumjohann, W., Barabash, S., and Andrè, N. and the MPO/SERENA, MPO-MAG, Mio-MGF, Mio/MPPE-MEA and MSA teams: Mercury’s Environment Observed by BepiColombo during the Second Mercury’s Swing-by, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10436, https://doi.org/10.5194/egusphere-egu25-10436, 2025.

EGU25-11316 | Posters on site | PS1.1

Ion species of Mercury’s 6th flyby, detected by PICAM's Hadamard mass spectrometry 

Ali Varsani, Helmut Lammer, Anna Milillo, Daniel Schmid, Daniel Heyner, Jim Raines, Gunter Laky, Norbert Krupp, Harald Jeszenszky, Gabriel Giono, Martin Volwerk, Daniel Teubenbacher, Rumi Nakamura, Stefano Orsini, Stefano Livi, Stas Barabash, Markus Fraenz, Harald Krueger, Alessandro Aronica, and Adrian Kazakov

BepiColombo, the joint ESA-JAXA mission on route to the planet Mercury, was launched in 2018. After eight successful planetary flybys, the spacecraft had its final Mercury flyby on 08 Jan 2025. The PICAM (Planetary Ion Camera) instrument, part of the SERENA package, was operational from 48 hours prior to the closest encounter, until 48 hours afterwards. This ion sensor successfully monitored the upstream solar wind, as well as the magnetospheric and planetary ions at the vicinity of Mercury. Near the planet, PICAM operated in mass spectrometry mode using its Hadamard Time-of-Flight gating, which is a novel technique to improve the observations of low-density ions. We present the analysis of the ion species detected at Mercury’s environment.

How to cite: Varsani, A., Lammer, H., Milillo, A., Schmid, D., Heyner, D., Raines, J., Laky, G., Krupp, N., Jeszenszky, H., Giono, G., Volwerk, M., Teubenbacher, D., Nakamura, R., Orsini, S., Livi, S., Barabash, S., Fraenz, M., Krueger, H., Aronica, A., and Kazakov, A.: Ion species of Mercury’s 6th flyby, detected by PICAM's Hadamard mass spectrometry, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11316, https://doi.org/10.5194/egusphere-egu25-11316, 2025.

EGU25-11550 | ECS | Orals | PS1.1

Investigation of the Low-Latitude Boundary Layer (LLBL) in Mercury's Magnetosphere 

Xue Wang, Lina Hadid, Sae Aizawa, Fouad Sahraoui, Jim Raines, and Benoit Lavraud

The MESSENGER spacecraft, which orbited Mercury from 2011 to early 2015, provided crucial insights into the structure and dynamics of Mercury's magnetosphere, including the identification of the Low Latitude Boundary Layer (LLBL). LLBL forms a mixed region of the magnetospheric and magnetosheath plasma, playing a crucial role in transferring mass and energy from the solar wind into the planetary magnetosphere. A statistical study by Liljablad et al. (2015) examined the properties of the LLBL during MESSENGER's first orbital year. More recently, the BepiColombo spacecraft crossed the LLBL in Mercury's duskside magnetosphere during its third Mercury flyby in 2023. Using the Mercury Plasma Particle Experiment (MPPE) instruments, specifically the ion analyzer (MIA) and mass spectrum analyzer (MSA), clear ion energy dispersion ranging from a few eV/e to 40 keV/e was observed (Harada et al., 2024; Hadid et al., 2024).

This study aims to build on these findings by conducting a comprehensive analysis of the LLBL using all MESSENGER data collected throughout its orbital period. The Magnetic field (MAG) and ion data (FIPS) revealed 351 LLBL cases. Considering the energy variation of the maximum differential flux of protons from the magnetopause toward the magnetosphere, 38 cases exhibited decreasing H⁺ energy dispersion, while 88 showed increasing H⁺ energy dispersion. Notably, the average H⁺ temperature is higher in LLBLs with increasing dispersion compared to those with decreasing or no dispersion. A clear dawn-dusk asymmetry was observed: 85% of H⁺ decreasing cases occurred on the duskside, while 89% of H⁺ increasing cases were on the dawnside.  Interestingly, in many LLBL cases, the energy dispersion of He²⁺ ions differed from that of H⁺, particularly in the majority of increasing cases, though He²⁺ data is limited. Following orbit insertion, the 3D distribution functions measured by the ion sensors (MIA and MSA) aboard the BepiColombo magnetospheric orbiter will enable a more detailed analysis.

How to cite: Wang, X., Hadid, L., Aizawa, S., Sahraoui, F., Raines, J., and Lavraud, B.: Investigation of the Low-Latitude Boundary Layer (LLBL) in Mercury's Magnetosphere, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11550, https://doi.org/10.5194/egusphere-egu25-11550, 2025.

EGU25-11718 | Orals | PS1.1

Ion observations and composition from MSA and MIA during BepiColombo's final gravity assist maneuver at Mercury 

Lina Hadid, Yuki Harada, and Yoshifumi Saito and the MSA/MPPE and MIA/MPPE teams
On January 8th, 2025, BepiColombo performed its sixth and final gravity assist maneuver (MFB6) at Mercury. This final maneuver followed the previous fourth flyby (MFB4), which was conducted in the polar regions. Unlike the first three flybys, which occurred near the equatorial regions, the spacecraft approached the planet from south to north, traveling from the nightside to the dayside across the cusp region at altitudes as low as ~265 km above the planet’s surface.
Although BepiColombo is in a "stacked configuration" during cruise (meaning that most of the instruments cannot be fully operated), several instruments remain capable of making valuable observations. In particular, despite their limited field of view, the particle sensors provide insights into the plasma composition and dynamics along a unique path across the magnetosphere, close to the planet. Notably, the Mass Spectrum Analyzer (MSA), part of the Mercury Plasma Particle Experiment (MPPE, PI: Y. Saito) consortium, detected clear evidence of Na+ ions and heavier ion species such as K+ around closest approach. In this presentation, we provide an overview of the ion observations from MSA and the Mercury Ion Analyzer (MIA), focusing on the ion composition during MFB6 in comparison with MFB4.

How to cite: Hadid, L., Harada, Y., and Saito, Y. and the MSA/MPPE and MIA/MPPE teams: Ion observations and composition from MSA and MIA during BepiColombo's final gravity assist maneuver at Mercury, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11718, https://doi.org/10.5194/egusphere-egu25-11718, 2025.

EGU25-11787 | ECS | Orals | PS1.1

Accelerated electrons in Mercury’s magnetosphere observed during the 3rd Mercury flyby of BepiColombo 

Sae Aizawa, Emilia Kilpua, Rami Vainio, Mathias Rojo, Nicolas Andre, Manuel Grande, Beatriz Sanchez-Cano, Marco Pinto, Yoshifumi Saito, and Fouad Sahraoui and the MEA-SIXS-PWI of BepiColombo

BepiColombo, launched in October 2018, is currently en route to Mercury. Although its planned orbit insertion is set for November 2026, BepiColombo continuously gathers new measurements during Mercury flybys. Throughout the cruise phase, the two spacecraft remain docked, with Mio protected behind the MOSIF sun shield, resulting in a limited observation for many instruments. Despite of such constraints, thanks to the smaller Larmor radii of electrons, wider range of electrons (from a few eV to a few hundreds of keV) got detected during the 3rd Mercury flyby by Mercury Electron Analyzer (MEA) onboard Mio and Solar Intensity X-ray and Particle Spectrometer (SIXS) onboard the Mercury Planetary Orbiter (MPO). Both instruments show quite similar variations indicating that they are observing same populations of electrons with wider energy range, and small differences in time indicate there are time-of-flight of electrons related to the drift motion of particles in the magnetosphere. Together with Plasma Wave Investigations (PWI) onboard Mio, the possible electron accelerations and transport will be discussed.

How to cite: Aizawa, S., Kilpua, E., Vainio, R., Rojo, M., Andre, N., Grande, M., Sanchez-Cano, B., Pinto, M., Saito, Y., and Sahraoui, F. and the MEA-SIXS-PWI of BepiColombo: Accelerated electrons in Mercury’s magnetosphere observed during the 3rd Mercury flyby of BepiColombo, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11787, https://doi.org/10.5194/egusphere-egu25-11787, 2025.

EGU25-11985 | Orals | PS1.1

 Mercury's Love number h2: Expected error range throughout the BepiColombo mission 

Oliver Stenzel, Martin Hilchenbach, Azar Arghavanian, and Haifeng Xiao

Introduction: Mercury, the innermost planet in the Solar System, remains an enigma due to significant gaps in our understanding of its internal structure. Recent advancements in planetary science have highlighted the potential of tidal Love numbers, specifically k2 and h2, to provide critical insights into the size of Mercury's inner core [1]. The Love number k2 represents a gravitational parameter, while h2 characterizes the radial deformation of the planet's surface. The determination of h2 can be achieved through techniques such as laser altimetry. The upcoming BepiColombo mission, set to arrive at Mercury in late 2026 [2], will enhance our understanding of Mercury's interior. A key instrument aboard BepiColombo, the Laser Altimeter (BELA), will enable the mapping of time-dependent surface elevations, providing crucial data for calculating h2 [3,4].

This study simulates BepiColombo's measurements using an orbit, observation, and tides model [5,6,7] to examine how the uncertainty in h2 decreases over the observation period. The BepiColombo Mercury Planetary Orbiter (MPO) offers significantly better coverage of Mercury's tidal potential compared to the MESSENGER mission [8,9], suggesting that the BepiColombo mission will yield more precise measurements of the h2 parameter. However, the simulation kernels used in this study are based on outdated mission parameters due to the revised arrival schedule of BepiColombo. To ensure the accuracy and relevance of our findings, we plan to update the simulations with the most recent kernel data.

To further explore the potential of the BepiColombo mission in constraining Mercury's internal structure, we will employ a simulation-based approach using planning kernels provided by the European Space Agency (ESA). Our model will simulate observations of Mercury's surface topography, incorporating tidal signals to model the planet's response to external gravitational forces. Additionally, observational errors and potentially different rotation states of Mercury will be introduced to reflect the expected noise levels from the BELA laser altimeter. These simulated observations will be used to calculate the Love number h2 and its associated uncertainty for different observation durations. This will allow us to assess how the mission's length influences the precision of the h2 measurement.

Acknowledgments: This work is supported by DLR under grant 50QW2301. PDS data used in this work: Neumann G. (2016), urn:nasa:pds:mess_mla_calibrated::1.0, 10.17189

References: [1] Steinbrügge G. et al. (2018), JGR, 123, 2760-2772. [2] Benkhoff J. et al. (2010), PSS, 58, 2-20. [3] Thomas N. et al. (2007), PSS, 55, 1398-1413. [4] Thomas, N. et al. (2021), Space Sci. Rev., 217. [5] Koch C. et al. (2010), PSS, 58, 2022-2030. [6] Thor R. N. et al. (2021), J. Geod., 95. [7] Thor R. N. et al. (2020), A&A, 633, A85. [8] Santo A.G. et al. (2001), PSS 49, 1481-1500. [9] Cavanaugh J.F. et al. (2007) Space Sci. Rev., 131, 451-479

How to cite: Stenzel, O., Hilchenbach, M., Arghavanian, A., and Xiao, H.:  Mercury's Love number h2: Expected error range throughout the BepiColombo mission, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11985, https://doi.org/10.5194/egusphere-egu25-11985, 2025.

EGU25-15163 | ECS | Orals | PS1.1

Energetic Electron Observations During BepiColombo’s First Three Mercury Flybys 

Liam Edwards, Manuel Grande, David Lawrence, Emilia Kilpua, Rami Vainio, Arto Lehtolainen, and Eero Esko

Mercury hosts a dynamic and highly variable magnetosphere shaped by its weak intrinsic magnetic field and the intense pressure of the solar wind. Previous observations from spacecraft sent to the planet have provided key insights into Mercury’s magnetospheric structure and energetic particle populations, revealing transient and highly variable energetic electron enhancements within the planet’s magnetosphere. We present BepiColombo/SIXS observations of energetic electron populations in Mercury’s magnetosphere during the spacecraft’s first three flybys of the planet. Although no such populations were observed during the first flyby, strong energetic electron signatures were observed during the second and third flybys. These observations are discussed in the context of observations by MESSENGER (Lawrence et al., 2015) in the invariant latitude-MLT plane, showing good agreement between the two data sets. Additionally, we present the highest time resolution energy spectra (> 70 keV) produced at Mercury during the second and third flybys.

How to cite: Edwards, L., Grande, M., Lawrence, D., Kilpua, E., Vainio, R., Lehtolainen, A., and Esko, E.: Energetic Electron Observations During BepiColombo’s First Three Mercury Flybys, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15163, https://doi.org/10.5194/egusphere-egu25-15163, 2025.

EGU25-15352 | Orals | PS1.1

Solar wind velocity reconstruction at Mercury using MESSENGER bow shock and magnetopause crossings.  

Daniel Heyner, Lars Klingenstein, Kristin Pump, Sae Aizawa, Daniel Schmid, and Ferdinand Plaschke

The solar wind significantly shapes and influences planetary magnetospheres, driving their structure and dynamics. Mercury, with its weak intrinsic magnetic field and close proximity to the Sun, is particularly sensitive to solar wind variations and adapts quickly to solar wind changes. Understanding solar wind characteristics, such as flow speed, is essential for fine-tuning magnetospheric models and eventually for interpreting Mercury’s magnetospheric response to solar wind changes. The solar wind speed affects both the aberration angle, which tilts the magnetosphere relative to the Mercury-Sun line, and the subsolar standoff distances from the internal dipole center of both the bow shock as well as the magnetopause.

This study reconstructs solar wind speeds from various bow shock and magnetopause crossings observed in-situ by MESSENGER’s magnetometer. We fit empirical bow shock and magnetopause models to the aberration angle and treat the subsolar standoff distances as additional parameters. For single crossings, a strong correlation between the parameters emerges. Thus, they cannot be independently determined, resulting in an infinite set of possible solutions for solar wind speed. To alleviate this problem, we combine multiple crossings to find a common aberration angle. Here, we present and discuss the first statistical results from the analysis and compare them to average boundary shapes and positions.

How to cite: Heyner, D., Klingenstein, L., Pump, K., Aizawa, S., Schmid, D., and Plaschke, F.: Solar wind velocity reconstruction at Mercury using MESSENGER bow shock and magnetopause crossings. , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15352, https://doi.org/10.5194/egusphere-egu25-15352, 2025.

EGU25-15727 | Orals | PS1.1

Laboratory Spectral Measurements to Simulate Pyroclastic Material on Mercury 

Alessandro Maturilli, Cristian Carli, Anna Galiano, Antti Penttilä, and Anna Irene Landi

The recognition of pyroclastic deposits on Mercury surface was driven by the presence of central pit (vent) surrounded by a spectrally bright and red deposit (facula) (Head et al, Science, 2008). In particular, the Visible to Near-InfraRed (VNIR) spectral properties permitted them to differentiate it from the surrounding terrains and defining the putative border of the deposits (e.g. Head et al, Science, 2008), since there is no morphological evidence that permits to limit their areal extension. Consequently, to improve our understanding of how the spectral properties of the effusive material extruded during the pyroclastic activity can change, considering variations in composition or textural properties of the material could improve our understanding of the pyroclastic deposits itself.

In this work we planned spectral analysis in reflectance and emittance of a systematic variation of samples with a silicate component as an example of pyroclastic extruded lava mixed with graphite or sulfide suitable for product formed with interaction of volatiles components during the pyroclastic activity at very reduced condition on Mercury (e.g., Cartier&Wood, Elements, 2019).

The pyroclastic endmember was prepared considering different variations among a crystalline mafic material and an amorphous component. We take into account variations in abundance as well as variation of particle size for the endmembers and for the mixtures.

All the samples have been measured in bidirectional reflectance in the VIS+VNIR+MIR spectral range, with particular attention to the 0.4-2.0 mm and 7-14 mm, spectral ranges where SIMBIO-SYS and MERTIS, onboard to Bepicolombo (Benkhoff et al., Spa.Sci.Rev., 2021), will operate. Moreover, for selected samples, emissivity (at Tsample = 150°, 250°, 350°, 450° C) in the MIR spectral range will be carried on. All the spectroscopic measurements are done at the PSL of DLR in Berlin.

This research was supported by the International Space Science Institute (ISSI), through International Team project #552 (Wide-ranging characterization of explosive volcanism on Mercury: origin, properties, and modifications of pyroclastic deposits).

How to cite: Maturilli, A., Carli, C., Galiano, A., Penttilä, A., and Landi, A. I.: Laboratory Spectral Measurements to Simulate Pyroclastic Material on Mercury, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15727, https://doi.org/10.5194/egusphere-egu25-15727, 2025.

EGU25-17082 | ECS | Posters on site | PS1.1

The role of mantle layering and mineralogical-dependent thermal properties on the evolution of Mercury's interior 

Manon Lécaille, Nicola Tosi, Olivier Namur, Attilio Rivoldini, and Bernard Charlier

Cooling and crystallization of Mercury's magma ocean likely formed a layered mantle composed of various proportions of minerals such as olivine, orthopyroxene, clinopyroxene, sulfides, and plagioclase, each with distinct thermal properties (e.g. thermal diffusivity, thermal conductivity, heat capacity, and melting temperature). Planetary thermal evolution models often consider an homogeneous mantle and treat these properties as constant or only varying with pressure and/or temperature. Their dependence on composition and modal proportions  is usually neglected, but can have a large impact on the modeled evolution.

Recent experimental studies gave access to the thermal conductivity and diffusivity of olivine, orthopyroxene and clinopyroxene. We calculated the thermal conductivity and diffusivity profiles of Mercury’s mantle assuming it is made of the Mg-rich endmembers forsterite, enstatite or diopside (i.e. the most likely phases occurring in the reduced interior of Mercury). We used a 1D parameterized model to simulate the thermal evolution of the planet with conductivity values varying from 1 to 4 Wm-1K-1, covering the above range of different mineralogies. We investigated several scenarios with (1) homogeneous conductivity over the whole mantle; (2) two layers characterized by different conductivity values. We then analyzed the results in terms of crust production and duration of mantle melting.

At pressures and temperatures relevant for Mercury's mantle, enstatite and diopside have higher conductivities and diffusivities than forsterite. This has a direct impact on the thermal evolution of the planet and on the melting of a fertile layer. Indeed, the more conductive the mantle is, the shorter its melting duration. Therefore, a mantle characterized by the conductivity of enstatite or diopside would promote a shorter melting time than one with conductivity of forsterite. In a two-layer mantle, melting duration is lower when conductivity of the top layer is higher compared to the bottom layer. The melting duration would thus be shorter for a mantle with a refractory olivine-like mantle conductivity at the base and an enstatite- and diopside-bearing fertile mantle-like conductivity in the upper part of the stratigraphic column. Besides the thermal conductivity, other parameters such as solidus temperature and heat production rate will be taken into account to obtain a consistent picture of the influence of mineralogical-dependent parameters on Mercury's evolution.

Accounting for variations in thermal conductivity and diffusivity due to heterogeneity in the mantle is therefore crucial in modeling planetary interiors. These factors significantly affect key parameters like crust thickness and the duration of volcanism.

How to cite: Lécaille, M., Tosi, N., Namur, O., Rivoldini, A., and Charlier, B.: The role of mantle layering and mineralogical-dependent thermal properties on the evolution of Mercury's interior, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17082, https://doi.org/10.5194/egusphere-egu25-17082, 2025.

EGU25-17383 | Orals | PS1.1

Planetary shadowing and Solar Energetic Particles during the fourth and sixth BepiColomo Mercury Flybys 

Emilia Kilpua, Rami Vainio, Manuel Grande, Liam Edwards, Eero Esko, Monica Laurenza, Arto Lehtolainen, Philipp Oleynik, Christian Palmroos, Scige John Liu, Stefano Massetti, and Daniel Heyner

The closest planet to the Sun, Mercury, is subject to particularly intense fluxes of solar energetic particles (SEPs). Its relatively weak magnetic field and small magnetosphere offer some protection againts these particles, deflecting them away before they can reach the surface. The effectiveness of this shielding could be probed in detailed during BepiColombo’s fourth (4 September 2024) and sixth (8 January 2025) flybys when and SEP events happened to be ongoing and the planet was immersed in high fluxes of energetic particles. During the fourth flyby, BepiColombo reached only 165 kilometres from the Mercury’s surface. In this presentation we analysis high energy electron and proton observations provided by the Solar Intensity X-ray and Particle Spectrometer SIXS. The data reveal a deep drop out in energetic particles fluxes due planetry shadowing. In addition, these unique measurements reveal that variations in particle fluxes depend clearly on particle type, direction and energy.

 

How to cite: Kilpua, E., Vainio, R., Grande, M., Edwards, L., Esko, E., Laurenza, M., Lehtolainen, A., Oleynik, P., Palmroos, C., Liu, S. J., Massetti, S., and Heyner, D.: Planetary shadowing and Solar Energetic Particles during the fourth and sixth BepiColomo Mercury Flybys, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17383, https://doi.org/10.5194/egusphere-egu25-17383, 2025.

EGU25-17874 | ECS | Orals | PS1.1

Spectral characterization of lab-made silicate glasses as analogues for Mercury: influence of grain size and chemical composition. 

Alessandro Pisello, Maximiliano Fastelli, Enrico Scricciolo, Marco Baroni, Alessandro Musu, Paola Comodi, and Diego Perugini

Volcanic and magmatic processes have played a significant role in shaping Mercury’s surface and contributing to its mineral diversity. Areas such as smooth plains, which cover 27% of the planet, are thought to have formed from effusive volcanic events. Explosive volcanism is also suggested by the presence of depressions surrounded by high-reflectance halos, calderas, and vents linked to impact structures or faults. The BepiColombo mission, a collaboration between ESA and JAXA, was launched in 2018 to explore Mercury. It consists of two orbiters, MIO (JAXA) and MPO (ESA), with a focus on studying the planet's interior, surface, exosphere, and magnetosphere. The MPO carries instruments such as SIMBIO-SYS and MERTIS, which are designed to acquire spectral data.

Interpreting planetary surface data often requires understanding complex factors like mineral composition, elemental abundance, temperature, and particle size. This study investigates the mid-infrared (MIR) spectral response of silicate glasses with a range of grain sizes and chemical compositions, aiming to build a database to support future spectral analyses of Mercury’s surface, where volcaniclastic materials are expected to be abundant.

Three compositions resembling the Northern Volcanic Plains (NVP) on Mercury were prepared: NVP, NVP_Na, and NVP_Mg, each with varying amounts of Na and Mg. These compositions were created by melting pure oxides at 1400°C, then crushing the resulting glass into powder and re-melting it to ensure homogeneity. The glass was sieved into various grain size fractions, with some samples mixed to create new samples with Gaussian-like distributions to explore how fine-grained fractions affect spectral responses, particularly in relation to volcanic ash.

Spectroscopic analysis was performed using a Bruker Invenio-X FT-IR spectrometer. The VNIR spectra (400-2000 nm) showed typical features of silicate glasses, with an absorption peak at around 1100 nm and a weaker one at 1900 nm, related to Fe-O bonds. The slope of the spectra did not vary much with increasing grain size in NVP samples, but there was a noticeable increase in the NIR slope (1200-1800 nm) for NVP_Na and NVP_Mg.

In the MIR region (7-14 µm), the spectra revealed a correlation between the shape of the spectra and the chemical and granulometric characteristics of the samples. A local maximum at 10000 nm was observed for all spectra, associated with tetrahedral silicate units, and the NVP_Mg spectra showed distinct features due to the network-modifying role of Mg. The spectra also exhibited the Christiansen Feature at around 8 µm, a diagnostic feature for igneous products, and a transparency feature around 12 µm, which appeared in spectra of finer-grained samples.

These spectra will be made available on the SSDC-ASI portal and will be crucial for interpreting data from the BepiColombo mission, particularly from SIMBIO-SYS and MERTIS. This research will help in identifying potential unknown igneous materials on Mercury’s surface.

How to cite: Pisello, A., Fastelli, M., Scricciolo, E., Baroni, M., Musu, A., Comodi, P., and Perugini, D.: Spectral characterization of lab-made silicate glasses as analogues for Mercury: influence of grain size and chemical composition., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17874, https://doi.org/10.5194/egusphere-egu25-17874, 2025.

EGU25-17931 | Posters on site | PS1.1

Comparative Analysis of Magnetic Field Observations during BepiColombo Mercury Flybys 

Daniel Schmid, Wolfgang Baumjohann, Ayako Matsuoka, David Fischer, Werner Magnes, Daniel Heyner, Hans-Ulrich Auster, and Rumi Nakamura

The BepiColombo mission, a collaboration between the European Space Agency (ESA) and the Japan Aerospace Exploration Agency (JAXA), aims to explore Mercury and its space environment. This mission is the first multi-spacecraft endeavor beyond Earth, comprising the Mercury Planetary Orbiter (MPO), managed by ESA, and Mio, led by JAXA. Launched in 2018, BepiColombo is still in cruise phase and recently completed its sixth and final swing-by maneuver at Mercury before its arrival in December 2026. This study provides a comparative analysis of magnetic field observations during the mission's Mercury flybys, utilizing data from the Magnetometer (MGF) onboard the Mio spacecraft. We aim to characterize the observed space environment and solar wind conditions for each flyby. The distinct flyby trajectories enable the exploration of extended regions around Mercury, encompassing the distant magnetotail, bow shock, and both hemispheres along the terminator. These observations provide valuable insights into the magnetospheric and solar wind conditions during each of the six flybys, significantly enhancing our understanding of the dynamic behavior of the solar wind in the inner heliosphere and the complex structure of Mercury's magnetosphere.

How to cite: Schmid, D., Baumjohann, W., Matsuoka, A., Fischer, D., Magnes, W., Heyner, D., Auster, H.-U., and Nakamura, R.: Comparative Analysis of Magnetic Field Observations during BepiColombo Mercury Flybys, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17931, https://doi.org/10.5194/egusphere-egu25-17931, 2025.

EGU25-17959 | ECS | Posters on site | PS1.1

Glinka crater on Mercury: a spectral and morphological analysis 

Mafalda Ianiri, Giuseppe Mitri, and Francesca Zambon

The surface of Mercury has been extensively altered by space weathering and impact processes, making it challenging to identify the boundaries of geological units. We analyzed the Glinka crater in the Beethoven quadrangle (H-07), a region characterized by notable spectral and geological variability, including impact craters, a possible pyroclastic vent, hollows, and compressive structures. To delineate morphological boundaries, we integrated high-resolution imaging, spectral data, and topographic products.

For morphological mapping, we produced monochromatic mosaics at 121 m/px, 56 m/px, and 14 m/px resolutions using MESSENGER MDIS/NAC data. Spectral investigations utilized an eight-filters MDIS/WAC-derived multispectral image (268 m/px). Additional datasets including Digital Elevation Model (DEM, 222 m/px), roughness and shading maps, and gravity data. Data processing involved the Integrated Software for Imagers and Spectrometers (ISIS3), applying the Kaasalainen-Shkuratov photometric correction model considering the parameters derived by Domingue et al. (2016). Spectral unit identification relied on four parameters: Reflectance at 750 nm (R750), Global Spectral Slope between 430 and 1000 nm (S430-1000), IR Slope ranging between 750 and 1000 nm (S750-1000), and UV Slope between 430 and 560 nm (S430-560). Threshold values for these parameters were determined through supervised k-means clustering (k=4), resulting in maps showing Regions of Interest (ROIs) for each spectral parameter. To combine all threshold values of the four parameters, an automated process generated a composite map with over 400 ROIs. Smaller ROIs (<15% of the average pixel count per ROI) were excluded, and those with similar values (∆10%) were merged iteratively, yielding seven final spectral units.

We are producing a geological map of the area by integrating data from the spectral map and high-resolution imagery. The spectral map highlights spectral variations and, in some cases, compositional differences. This integration enables a more precise definition of the boundaries between geological units. involves detailed geological and chronostratigraphic interpretations involves the exploration of various RGB combinations to extract additional information. This analysis includes spectral parameter values for each unit, taking into account surface morphology and texture, which may influence spectral responses without necessarily indicating compositional differences.

Domingue D. L. et al. (2016) Icarus 268, 172-203. https://doi.org/10.1016/j.icarus.2015.11.040

 Acknowledgements:  M.I. and G.M. acknowledges support from the Italian Space Agency (2022-16-HH.1-2024).

How to cite: Ianiri, M., Mitri, G., and Zambon, F.: Glinka crater on Mercury: a spectral and morphological analysis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17959, https://doi.org/10.5194/egusphere-egu25-17959, 2025.

EGU25-18018 | Orals | PS1.1

Overview and initial results of BepiColombo Mercury flybys 

Go Murakami and Geraint Jones

The ESA-JAXA joint mission BepiColombo is still on the track to Mercury. The two spacecraft for BepiColombo, Mio (Mercury Magnetospheric Orbiter: MMO) and Mercury Planetary Orbiter (MPO), are combined with MMO Sun Shield (MOSIF) and Mercury Transfer Module (MTM) during the cruise phase. BepiColombo will arrive at Mercury in November 2026, and it has 8-years cruise with the heliocentric distance range of 0.3-1.2 AU. The long cruise phase also includes 9 planetary flybys: once at the Earth, twice at Venus, and 6 times at Mercury. On 8 January 2025 we completed the last (6th) Mercury flyby successfully. Even before arrival, we already obtained fruitful science data from Mercury during the Mercury flybys. We performed science observations with almost all the instruments onboard Mio and successfully obtained comprehensive data of Mercury’s magnetosphere such as magnetic fields, plasma particles, and waves. Here we present the overview and initial results of the science observations during the Mercury flybys.

How to cite: Murakami, G. and Jones, G.: Overview and initial results of BepiColombo Mercury flybys, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18018, https://doi.org/10.5194/egusphere-egu25-18018, 2025.

EGU25-18729 * | Orals | PS1.1 | Highlight

BepiColombo's Journey to Mercury: Lessons from Cruise Operations and Plans for Orbital Science 

Stavros Kotsiaros, Geraint Jones, Johannes Benkhoff, Santa Martinez Sanmartin, Sebastien Besse, David Frew, Paolo Cappuccio, Ines Belgacem, and Bernhard Geiger

The BepiColombo mission, a cornerstone of the European Space Agency's (ESA) Cosmic Vision program in collaboration with the Japan Aerospace Exploration Agency (JAXA), represents an ambitious endeavor to deepen our understanding of Mercury. It uniquely combines the Mercury Planetary Orbiter (MPO) and the Mercury Magnetospheric Orbiter (Mio) to investigate Mercury’s interaction with the solar wind, its geological history, and its magnetic environment. The mission seeks to address fundamental questions about the evolution of terrestrial planets, including Mercury’s formation, internal structure, and enigmatic magnetic field.

BepiColombo’s operational phase at Mercury will prioritize the implementation of a meticulously designed strategy to maximize the scientific potential of its complementary payload. The dual-spacecraft configuration enables synchronized observations of the planet’s surface, exosphere, and magnetosphere, offering unprecedented insights into the planet’s complex environment. Key mission strategies include utilizing the spacecraft’s elliptical orbits to optimize coverage during perihelion passes, supporting high-resolution investigations of regions of particular scientific interest, and facilitating comprehensive global mapping. These efforts aim to provide a holistic understanding of Mercury’s geological and magnetic properties, as well as its interactions with the solar wind, making significant contributions to planetary science.

This presentation will highlight the broader implications of BepiColombo’s mission design, the operational strategies planned for the science phase, and the valuable insights gained from its Venus and Mercury flybys. Particular focus will be placed on how these lessons refine the mission’s science objectives and influence future exploration initiatives targeting Mercury and other inner Solar System bodies.

How to cite: Kotsiaros, S., Jones, G., Benkhoff, J., Martinez Sanmartin, S., Besse, S., Frew, D., Cappuccio, P., Belgacem, I., and Geiger, B.: BepiColombo's Journey to Mercury: Lessons from Cruise Operations and Plans for Orbital Science, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18729, https://doi.org/10.5194/egusphere-egu25-18729, 2025.

EGU25-19385 | Orals | PS1.1

BepiColombo Mission Update 

Geraint H. Jones and Go Murakami

BepiColombo is a joint mission between the European Space Agency (ESA) and the Japanese Aerospace Exploration Agency (JAXA), which will carry out the comprehensive exploration of planet Mercury. The mission was launched on 20 October 2018 from the European spaceport Kourou in French Guiana, and is currently on a eight-year-long cruise to Mercury. BepiColombo consists of two orbiters, the Mercury Planetary Orbiter (MPO) and the Mercury Magnetospheric Orbiter (Mio). In late 2026, these orbiters will be put in orbit around the innermost planet of our Solar System. Once in orbit, BepiColombo with its state of the art and very comprehensive payload will perform measurements to increase our knowledge on the fundamental questions about Mercury’s evolution, composition, interior, magnetosphere, and exosphere. BepiColombo successfully completed the last of its 6 flybys of Mercury in January 2025, and will continue its cruise during the rest of 2025 and much of 2026. Although the two BepiColombo orbiters are in a stacked configuration during the cruise, during which only some of the instruments can perform scientific observations, the mission has already produced some very valuable results, as well as striking observations of the planet using its three engineering monitoring cameras. We shall provide a summary of the mission status, a preview of the remaining plans for the mission up to and after arrival in orbit around Mercury, a broad overview of scientific results to date, and observations by the mission's monitoring cameras from the Mercury flybys.

How to cite: Jones, G. H. and Murakami, G.: BepiColombo Mission Update, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19385, https://doi.org/10.5194/egusphere-egu25-19385, 2025.

EGU25-19661 | ECS | Posters on site | PS1.1

Laboratory simulation of ion impact and back-scattering on Mercury surface analogues for planetary space weather investigation 

Alessandro Brin, Grace Richards, Elisabetta De Angelis, Rosanna Rispoli, Martina Moroni, Roberto Sordini, Luca Colasanti, Nello Vertolli, Fabrizio Nuccilli, Alessandro Mura, Valeria Mangano, Stefano Orsini, Christina Plainaki, and Stefano Massetti

Mercury has a surface-bound exosphere that mediates transport of ion and netural species on the surface and within the Hermean environment. When precipitating solar wind particles impact the planet’s regolith, ions may be neutralised and backscattered, form chemical reactions with surface species, or induce sputtering processes. The SERENA (Search for Exospheric Refilling and Emitted Neutral Abundances) instrument onboard BepiColombo aims to study these surface-exosphere-magnetosphere interactions, using a suite of particle detectors and mass spectrometers. 
At INAF/IAPS, the Ion and Energetic Neutral Atom (I-ENA) laboratory facilitates controlled experiments on the interaction of ion/neutral beams with diverse surface analogues and detectors for planetary space weather investigation. ELENA (Emitted Low Energy and Neutral Atoms) one of the SERENA instruments, is devoted to detect backscattered ENA and possibly magnetospheric and solar wind ions with an energy range of 10 eV-5 keV, and its Flight Spare (FS) is tested and calibrated in the laboratory. The ELENA FS is intended to be used for future investigations of backscattering process with Mercury analogues. Laboratory experiments involving irradiation of Mercury analogues aim to provide ground truth to the data provided by this instrument. 
We present a test for simulating Solar Wind interactions with Mercury surface analogues. Mercury analogues are placed in a bespoke vacuum system which achieves working pressures of 10-7 mbar. A particle beam of energies between 0.5-5 keV (Helium-Argon), that can be modulated in intensity, area and direction, is used to irradiate samples. The charged particle beam (ions) can also be made into a beam of ENA with a neutralisation cell for charge exchange effect. 
We plan to investigate a variety of diverse samples, including slabs of meteorite and pellets similar in composition and grain size to Mercury’s surface.
This work will provide a detailed description of the facility and experimental framework, while identifying open questions and fostering discussions on interdisciplinary collaborations needed to advance Mercury science. Such experiments are pivotal for improving our understanding of Mercury’s environment and directly support the goals of the BepiColombo mission.

How to cite: Brin, A., Richards, G., De Angelis, E., Rispoli, R., Moroni, M., Sordini, R., Colasanti, L., Vertolli, N., Nuccilli, F., Mura, A., Mangano, V., Orsini, S., Plainaki, C., and Massetti, S.: Laboratory simulation of ion impact and back-scattering on Mercury surface analogues for planetary space weather investigation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19661, https://doi.org/10.5194/egusphere-egu25-19661, 2025.

EGU25-21593 | ECS | Orals | PS1.1

A snapshot of Mercury’s magnetosphere seen by MIPA in BepiColombo’s MSB6 

Hayley Williamson, Stas Barabash, Martin Wieser, Hans Nilsson, Yoshifumi Futaana, Anna Milillo, Alessandro Aronica, Adrian Kasakov, Stefano Orsini, Ali Varsani, and Gunter Laky

BepiColombo made its sixth and final swing-by of Mercury on January 8, 2025, crossing from the nightside over the north pole to the dayside near the noon-midnight plane. The Miniature Ion Precipitation Analyzer (MIPA), an ion analyzer in the Search for Exospheric Refilling and Emitted Natural Abundance (SERENA) instrument suite on the Mercury Planetary Orbiter (MPO), made observations throughout the swing-by, observing positive ions in the range from 30 eV – 14 keV with a hemispherical field of view. This swing-by gives a unique snapshot of the state of Mercury’s magnetosphere, as MIPA observed several magnetospheric regions within a short period, some of them for the first time. We observe the plasma sheet and plasma sheet horns, as well as plasma upwelling from the northern polar cusp to the dayside magnetopause. Passing through the dayside magnetosheath shows high anisotropic fluxes, as the magnetosheath bulk flow was in the MIPA FOV, unlike previous swing-bys. Following the bow shock crossing, we see a distinct foreshock population, followed by a half an hour gap in signal before a second foreshock detection at +5 RM. We then compare the MIPA observations to modeled magnetic fields and environment. The combination of all the swing-bys highlights the versatility of planetary swing-by trajectories, which allow for observations of regions that may not be accessible after orbit insertion.

How to cite: Williamson, H., Barabash, S., Wieser, M., Nilsson, H., Futaana, Y., Milillo, A., Aronica, A., Kasakov, A., Orsini, S., Varsani, A., and Laky, G.: A snapshot of Mercury’s magnetosphere seen by MIPA in BepiColombo’s MSB6, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21593, https://doi.org/10.5194/egusphere-egu25-21593, 2025.

EGU25-21600 | ECS | Posters on site | PS1.1

Statistical Analysis of Mercury’s Magnetic Cusp and its Dependence on Solar Wind Conditions 

Robin Zywczok and Daniel Heyner

The relationship between Mercury’s magnetic cusp and variations in the solar wind has been investigated in several prior studies. Building on this foundation, we developed an integrated approach that combines two independent detection algorithms: one that identifies cusp signatures using magnetic field data—based on magnetic anisotropy and angular variations relative to the KTH reference model (without the cusp)—and another that analyzes particle data, utilizing a method established by Jim Rains. A key aspect of this work is the comparison of these two independent detection methods to gain deeper insights into cusp behavior. Using this combined approach, we conducted a statistical analysis that reveals how the structure and occurrence of Mercury’s magnetic cusp vary under different solar wind conditions.

How to cite: Zywczok, R. and Heyner, D.: Statistical Analysis of Mercury’s Magnetic Cusp and its Dependence on Solar Wind Conditions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21600, https://doi.org/10.5194/egusphere-egu25-21600, 2025.

EGU25-3546 | ECS | Posters on site | HS1.2.2

Innovative Lagrangian Radiosonde Clusters for ABL Observations 

Shahbozbek Abdunabiev, Niccolo' Gallino, and Daniela Tordella

We present a novel method to track fluctuations in the atmospheric boundary layer (ABL) using a cluster of mini-radiosondes. Each radiosonde is lightweight, expendable and carried by biodegradable balloons. This system collects statistics of turbulence fluctuations in the ABL and warm clouds within it. The first operational prototype of the radiosonde cluster developed at POLITO was tested in several field campaigns from November 2022 to September 2024. These campaigns, which included six cluster launch experiments, were conducted in collaboration with CNR-INRIM, MET-OFFICE, NCAS, ARPA Piemonte, ARPA-FVG, and OAvdA (see Fig. 1). The system provides critical insights for modeling ABL dynamics and dispersion, a major source of uncertainty in climate and meteorological simulations [1].

Figure 1: In-field experiments with the radiosonde cluster network. LoRa P2P radio transmission, 12 km range, 868 MHz, 0.2 Hz data acquisition frequency. Left: radiosonde trajectories. Middle: vertical profiles of temperature and mean Brunt-Vaisala frequency from 3 radiosondes. The purple color indicates positive temperature gradients, while green indicates negative ones. Right: wind speed, magnetic field, and acceleration fluctuation spectra. A) Alpine environment, St. Barthelemy, Aosta, Italy, November 2023. B) Rural near-maritime Atlantic coast, Chilbolton, UK, July 2023, WESCON campaign. C) Subalpine region, Udine, Italy, June 2024. D) Rural near-maritime Atlantic coast, Chilbolton, UK, September 2024. Ground-level wind speeds: A: 1 m/s, B: 17 m/s, C: 0.5 m/s, D: 10 m/s.

Each radiosonde is a radioprobe board [1, 2] mounted on a biodegradable balloon [3] filled with a helium-air mixture, allowing a float time of several hours. It measures air temperature, pressure, humidity, and four vector quantities (position, velocity, acceleration, and Earth's magnetic field) along each trajectory (Fig. 1). Passive tracking of multiphase cloud parcels provides a multi-point view of flow structures. Recent experiments have explored turbulent dispersion analysis using a distance neighbor graph algorithm [4], addressing aspects of atmospheric turbulence not previously measured in field observations. The system can advance models for cloud microphysics and turbulence schemes for atmospheric tracer dispersion [5]. Our methodology uses high-frequency atmospheric data and improves understanding of turbulence. This enables advances in cloud modeling, weather prediction, and climate simulation. The biodegradable balloon has a volume of ~40 liters and weighs ~18 grams. Optimizing the size and weight of the circuit board (halving both dimensions) will reduce the balloon volume by 30%, allowing for simultaneous deployment of swarms of ~100 mini-radiosondes. The future radioprobe will have sensors for VOCs, greenhouse gases, and UV radiation integrated into the PCB to expand its use cases. An energy harvesting module will extend the lifetime of the probe.

1. Abdunabiev S. et al., Measurement 224, 113879 (2024)

2. Paredes et al., Sensors 21, 1351 (2021)

3. Basso et al., Mat. Chem. Phys. 253, 123411 (2020)

4. Richardson, Proc. R. Soc. Lond. A 110, 709 (1926)

5. Mirza et al., Q. J. R. Meteorol. Soc. 150, 761 (2024)

How to cite: Abdunabiev, S., Gallino, N., and Tordella, D.: Innovative Lagrangian Radiosonde Clusters for ABL Observations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3546, https://doi.org/10.5194/egusphere-egu25-3546, 2025.

EGU25-3756 | Posters on site | HS1.2.2 | Highlight

Sampling spores and microorganisms in the stratosphere 

Jérôme Kasparian, Sara Leoni, Océane Devisme, Maxime Hervo, Gonzague Romanens, and Katia Gindro

Spores are the survival and dissemination units of fungi. Many are designed for optimal airborne dispersal while maintaining long-term survival. Depending on the chemical and structural nature of their walls, they are highly resistant to extreme temperatures and UV radiation. For example, Botrytis cinerea conidia stored dry at -80°C are still able to germinate after more than 20 years in storage. Given their anemochorous nature and resistance to abiotic factors, it would therefore be possible for spores of pathogenic fungi to be aeroported through the stratosphere. However, little is known about the spread of pathogenic fungi in high-altitude airspace.

 

In order to investigate the presence of fungal spores in the stratosphere and explore the diversity of viable and non-cultivable fungi, we designed a low-cost sampling device capable of sampling particles in the stratosphere. It consists in a sealed polystyrene box with two ports on the top and bottom sides, allowing air circulation. A rotating arm sampler spins in the resulting airflow, with four sticks coated with petroleum jelly. The opening of the ports is controlled by mobile covers driven by servomotors, managed by an Arduino Uno microcontroller connected to a high-pressure pressure sensor. Moreover, an on-board radiosonde continuously transmits GPS position, relative humidity, and temperature data. An internal camera captures the opening, closing, and sampling processes during the desired altitude segment. Additionally, a control box, that never opens during flight,  monitors potential contamination below the stratosphere.

 

Both the measurement and control boxes are sterilized under UV-C, sealed and attached to a meteorologic radiosonding balloon. Upon reaching an altitude of 12,000 meters, the covers open, and airborne particles are collected. Once the balloon bursts (at around 35,000 m; -63°C), a parachute deploys during the descent, and the cover closes at 12,000 meters.  The prompt recovery of the sample at landing is assisted by a specifically dedicated mobile app, that extrapolates the descent trajectory and guides the crew to the expected landing location.

 

Five test flights between October 2023 and June 2024 up to 35,000 meters altitude, allowed us to optimize and validate the device, the sampling conditions, and the sample recovery procedures and analysis. The collected samples were both cultured on fungal medium and prepared for deep DNA sequencing. The control box remained sterile, confirming the absence of contamination. Furthermore, several species of cultivable fungi were identified in the sample, demonstrating the viability of spores despite low pressure and temperature, while the DNA sequencing revealed the presence of many species, including exotic ones.

 

This setup opens the way to routine monitoring of stratospheric airborne fungi spores and other biological aerosols, in view of a better understanding of their dispersal and survival.

How to cite: Kasparian, J., Leoni, S., Devisme, O., Hervo, M., Romanens, G., and Gindro, K.: Sampling spores and microorganisms in the stratosphere, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3756, https://doi.org/10.5194/egusphere-egu25-3756, 2025.

EGU25-12080 | Posters on site | HS1.2.2

Cryoegg, Cryowurst and Hydrobean: wireless instruments for glaciology and hydrology 

Michael Prior-Jones, Hawkins Jonathan, Lisa Craw, Elizabeth A Bagshaw, Christine F Dow, Allan Mason-Jones, Hashem Alnader, Elena von Benzon, Luke Copland, Dorthe Dahl-Jensen, Brittany Main, Josh James, Stephen Livingstone, Sarah Mann, Matthew Peacey, Rupert Perkins, and Sophia M Rahn

Observations of conditions within and beneath the ice of glaciers and ice sheets are required to better constrain models of glacier dynamics and provide more reliable forecasts of how ice responds to a changing climate. We have developed and deployed two wireless instruments intended to provide long-term observations of englacial and subglacial environments.  A third instrument has been developed for use in streams and rivers – this may be used in either glacial or temperate environments.

Cryoegg is a spherical instrument deployed in subglacial channels via boreholes, or in moulins. It measures temperature, water pressure and electrical conductivity and provides data live by radio link through the ice to a receiver on the surface. The spherical shape allows it to travel within water channels and report on conditions within the hydrological system. We demonstrate how it has provided 5 months of data from within a glacier moulin in west Greenland, and that the radio link can operate through 2,500m of ice in north-east Greenland.

Cryowurst is a cylindrical instrument deployed in a borehole and measures both subglacial hydrological parameters (water pressure, temperature and electrical conductivity) but also its tilt and orientation change as the ice moves. It also reports wirelessly to a datalogger on the glacier surface. It has provided 5 months of data during a deployment in Yukon, Canada.

Hydrobean is an instrument intended for citizen scientists studying streams and small rivers in temporate regions. It shares some common technology with the two cryospheric instruments. Hydrobean consists of a hemispherical unit deployed on the river bed, which sends data by radio link to a data logger on the bank. It measures water pressure, water temperature and electrical conductivity and is intended to help identify pollution events (which may raise both the temperature and electrical conductivity of the water). Hydrobean has been tested in the River Usk in Wales and the river Dart in south-west England. We also intend to deploy Hydrobean in supraglacial streams during future glaciological fieldwork.

The data loggers which receive the data from all three wireless instruments store the data locally but can also forward data to a web portal using cellular or satellite links. This has allowed us to closely monitor and retrieve data in close to real time and reduces the risk of data loss from equipment damage in a harsh environment.

How to cite: Prior-Jones, M., Jonathan, H., Craw, L., Bagshaw, E. A., Dow, C. F., Mason-Jones, A., Alnader, H., von Benzon, E., Copland, L., Dahl-Jensen, D., Main, B., James, J., Livingstone, S., Mann, S., Peacey, M., Perkins, R., and Rahn, S. M.: Cryoegg, Cryowurst and Hydrobean: wireless instruments for glaciology and hydrology, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12080, https://doi.org/10.5194/egusphere-egu25-12080, 2025.

EGU25-13702 | ECS | Posters on site | HS1.2.2

SPYCE: A Multi-Modal Rodent Monitoring Device for Enhanced Detection, Monitoring, and Behavior Analysis 

Chirag Padubidri, Ioannis Louloudakis, Ioannis Daliakopoulos, Sukru Esin, and Andreas Kamilaris

Rodents pose a significant threat to agriculture, causing extensive damage to crops, infrastructure, and ecosystem health. This pressing issue necessitates innovative, sustainable management solutions. SPYCE, a rodent-monitoring device (RMD), is designed to provide a flexible, adaptable solution for rodent detection, monitoring, and behavior-analysis. Developed as part of the MED4PEST project, which focuses on advancing ecologically based rodent management by reducing reliance on synthetic pest-control methods and promoting sustainable, eco-friendly farming systems tailored to the Mediterranean-region. SPYCE’s modular, customizable configuration allows users to select sensors based on operational requirements and budget constraints, emphasizing open accessibility, tailored functionality, and cost-effective deployment.


SPYCE is a T-shaped device designed for flexible deployment at greenhouse entry points and fenced agricultural fields. Its design allows rodents to enter and exit freely, facilitating precise monitoring. The T-joint structure includes a horizontal base pipe equipped with PIR sensors at each entrance to detect movement. A housing at the top of the vertical pipe contains critical sensors such as an ultrasonic sensor, ultrasonic microphone, and infrared camera oriented downward toward the T-joint, all integrated with a Raspberry-Pi. A mmWave-radar sensor monitors external movement signatures. A temperature-humidity sensor collects environmental data, while a protective top cover shields the electronics from dust and water.

The system firmware, developed in Python, supports three operational modes for various monitoring needs. In Mode-1, PIR sensors at the entrances activate the system, which waits for ultrasonic-sensor confirmation to initiate data collection. In Mode-2, the ultrasonic sensor detects motion at the central joint, directly triggering data acquisition. In Mode-3, the infrared camera operates continuously, detecting motion through background changes and activating other sensors when a rodent is detected. Across all modes, temperature-humidity data are recorded at regular intervals. Additionally, separate code records movement signatures using the mmWave radar. SPYCE’s modular design adapts to diverse operational requirements while maintaining accuracy and reliability in data collection. Furthermore, SPYCE is open-source, with hardware designs, scripts, and implementation details available on GitHub (https://github.com/superworld-cyens/MED4PEST), enabling researchers and practitioners to replicate and customize SPYCE for rodent monitoring.

SPYCE is currently deployed at pilot sites in Greece and Turkey, actively collecting rodent-activity data. This data will serve as the foundation for developing a multi-modal deep-learning model capable of detecting, counting, and analyzing rodent behavior with high precision. Additionally, multi-modal anomaly-detection techniques will investigate behavioral changes in rodents under EBRM and non-EBRM conditions, providing valuable insights. These pilot deployments will validate SPYCE’s potential as an effective tool for assessing EBRM strategies. This work can also extend to broader rodent-management applications, including population estimation, behavioral analysis, and ecological monitoring.

Funding: This work is part of MED4PEST, funded under the PRIMA Programme, an Art.185 initiative co-funded by Horizon-2020, the EU’s Research and Innovation Programme. Additional funding was provided by the General Secretariat for Research and Innovation, Greece; the Scientific and Technological Research Council of Turkey; the EU Horizon-2020 Research and Innovation Programme (grant No. 739578); and the Government of the Republic of Cyprus through the Directorate General for European Programmes, Coordination, and Development.

How to cite: Padubidri, C., Louloudakis, I., Daliakopoulos, I., Esin, S., and Kamilaris, A.: SPYCE: A Multi-Modal Rodent Monitoring Device for Enhanced Detection, Monitoring, and Behavior Analysis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13702, https://doi.org/10.5194/egusphere-egu25-13702, 2025.

EGU25-14559 | ECS | Posters on site | HS1.2.2

The Open Digital Environmental Lab 

Elad Levintal, Elyasaf Freiman, Thi Thuc Nguyen, Devi Orozco, Tom Norman, Robel Kahsu, and Ariel Altman

The development of new affordable sensors, and the ability to log high-resolution data for long periods of time can potentially revolutionize environmental sciences. Collecting high-resolution spatiotemporal data requires sensor grids that are often costly and not necessarily modular enough to fit a specific experimental objective. These are limiting factors that can be solved using open-source hardware. In our Open Digital Environmental Lab, we develop and integrate complex sensor arrays into our research that simultaneously measure multiple parameters, such as water content and CO2  and O2  concentrations. We rely on integrating IoT (Internet of Things) concepts and aim to meet not only our current research goals, but also to enable new capabilities at a fraction of traditional sensor costs but with similar accuracy. Our vision is that open-source sensors will: (1) “Democratize science” by reducing cost limitations, and (2) Be game-changers for measuring environmental parameters with the ability to capture process-related heterogeneity. At the conference, we will present various projects, ranging from lab-oriented devices to field networks for real-time monitoring of soil and river parameters that allow new modeling and mechanistic understandings.

How to cite: Levintal, E., Freiman, E., Nguyen, T. T., Orozco, D., Norman, T., Kahsu, R., and Altman, A.: The Open Digital Environmental Lab, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14559, https://doi.org/10.5194/egusphere-egu25-14559, 2025.

EGU25-18431 | Posters on site | HS1.2.2

Open Hardware in the UK Floods and Droughts Research Infrastructure (FDRI) 

Wouter Buytaert, Alejandro Dussaillant, and Will Veness

The UK Floods and Droughts Research Infrastructure (FDRI) is a £38 million investment from the UK Government to support transformative research and applications on flood and drought resilience. The infrastructure will consist of a combination of in-situ monitoring infrastructure, an overarching digital infrastructure to support telemetry, analytics, and data integration, and an extensive portfolio of capacity development, training and community building activities.

FDRI aims to be a state-of-the-art infrastructure that supports transformative research. This means that innovation sits at the heart of the infrastructure – both technological innovation using novel and emerging technologies, but also social innovation to explore novel arrangements for data collection, analysis, and knowledge co-production.

Open hardware provides unprecedented opportunities to support such innovation, not only as a source of new sensing and data processing technologies and setups, but also as a catalyst for engaging makers, inventors, entrepeneurs, citizen scientist and other innovation communities in FDRI.

Here we give an overview of the vision and implementation strategy of FDRI, as well as the specific opportunities for engagement, from early experimentation and prototyping to contributing to designing for cost-effectiveness, accuracy, robustness, longevity and long-term sustainability.

How to cite: Buytaert, W., Dussaillant, A., and Veness, W.: Open Hardware in the UK Floods and Droughts Research Infrastructure (FDRI), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18431, https://doi.org/10.5194/egusphere-egu25-18431, 2025.

EGU25-18763 | ECS | Posters on site | HS1.2.2

Automated wetting of a fiber-optic cable for forest evaporation partitioning 

Gijs Vis and Miriam Coenders-Gerrits

Measuring evaporation through Bowen ratios requires measuring a wet and a dry air temperature, something that is challenging to reliably accomplish in outdoor field conditions. In the context of forest evaporation, the desire to estimate Bowen ratios as a function of height (e.g., to partition evaporation above and below the canopy) adds another dimension of complexity to this measurement challenge.

As part of the Ruijsdael Observatory in the Loobos, Netherlands, we aim to continuously measure evaporation throughout a forest profile, using a dry and a wetted fiber-optic table along a 40 m tower to measure temperature profiles using Distributed Temperature Sensing (DTS). Previous studies have used continuous pumping with relatively large flow rates to ensure wetness, but this is not feasible for long term installations because of large water volume requirements.

In this contribution a smart and open-source solution for keeping a wet temperature wet and a dry temperature dry over a 40 m profile is presented. Two peristaltic pumps are regulated using two microcontrollers that modulate the pumping rate along different environmental conditions. For instance, no pumping could be needed at nighttime since there is negligible evaporation and pumping is stopped at low temperatures to prevent frost damage. A capacitive method is presented to attempt to quantify wetness, tank levels are monitored, and solutions for recycling water to limit the water volume requirements are introduced. Microcontrollers are connected to WiFi to enable convenient monitoring from the office.

With this contribution we hope to contribute to generalized solutions to measure evaporation or, in general, to inspire on methods about how to keep hydrological sensors wet or dry.

How to cite: Vis, G. and Coenders-Gerrits, M.: Automated wetting of a fiber-optic cable for forest evaporation partitioning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18763, https://doi.org/10.5194/egusphere-egu25-18763, 2025.

EGU25-19559 | ECS | Posters on site | HS1.2.2

Signal Transmission from the Water Surface for Plastic Pollution Tracking 

Marc Schneiter, Rolf Hut, and Erik Van Sebille

We use surface drifters to sample individual traces of floating macro plastic. These in-situ measurements provide input for the development of Lagrangian simulations to analyze both the dispersion patterns, and the physical transport processes of the plastic. An important component of drifters is the transmission of data directly from the water surface. This is challenging both due to the remoteness of the locations where the transmissions take place, and due to the dynamical movement of the water, which impedes signal transmission. For this reason, expensive satellite modems are often used, with careful design considerations that make the communication possible. The aims of our current research project are twofold: We want to test established and alternative terrestrial communication technologies at tens of kilometers from shore, and extend the knowledge about these data transmissions in challenging environments. This is done with a custom waterproof instrument that can be deployed and kept next to a research vessel. The instrument contains transition modems for satellite, cellular and LoRa communication. We present the construction of the instrument and results of a recent measurement campaign in the North Sea, off the Dutch coast.

How to cite: Schneiter, M., Hut, R., and Van Sebille, E.: Signal Transmission from the Water Surface for Plastic Pollution Tracking, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19559, https://doi.org/10.5194/egusphere-egu25-19559, 2025.

EGU25-1067 | ECS | Orals | SSP3.8

Multiproxy evaluation of the Paleohydrology of the Sakarya River during the Last Milennium, NW Anatolia 

Hilal Okur, Mehmet Korhan Erturaç, Meltem Çelen, Eren Şahiner, Zeki Bora Ön, Sena Akçer Ön, Nesibe Köse, Hüseyin Tuncay Güner, Nurgül Karlıoğlu Kılıç, and Mehmet Salim Öncel

Paleohydrology studies are an emerging field of research linked to paleoclimatology and hazard estimation studies. Understanding the patterns of extreme events in the context of global change is of great importance, especially for regions where extreme events are an integral part of the hydrological regime, due to their social (e.g., vulnerability) and political (resilience and adaptation) implications. For many regions of the world where the instrumental record is very short and there are no historical records of hydrological events. These instrumental records can be extended by hundreds to thousands of years by reconstructing especially paleoflood events using fluvial archives.

We present the first detailed paleohydrology study in Anatolia. Our research focuses on the lower reaches of the Sakarya River at Adapazarı Basin, NW Anatolia, Türkiye. Here, the due unique tectonic setting controlled by the North Anatolian Fault, deposition of a 4.5-meter-thick fine-grained floodplain sediment since CE 1350 was possible. This timing constraint corresponds to the reign of the Ottoman Empire as well as to the Little Ice Age (LIA), an intermitted period(s) of cold and dry climate defined for the northern Europe. The characterization of past flow regimes of the river and the detailed identification of paleohydrology events within the studied section have been facilitated through a multidisciplinary and multi-proxy approach (grain size, mineralogy, geochemistry). All identified events have been precisely dated using age-depth model based on dendrochronology, radiocarbon, luminescence, and event-based dating techniques.

The focus sedimentary record revealed that the Sakarya River experienced distinct long-duration regular flow and drought episodes with intermittent flooding events for the last 600 years. Within this time frame, with intervals of uncertainty, three dry and three regular hydrological regimes have been identified from the year CE 1350 to 1950. Within these hydrological regimes, 9 periods of extreme drought and 10 flood events have been identified. These episodes are closely comparable with the published local and regional paleo-climatic record.

How to cite: Okur, H., Erturaç, M. K., Çelen, M., Şahiner, E., Ön, Z. B., Akçer Ön, S., Köse, N., Güner, H. T., Karlıoğlu Kılıç, N., and Öncel, M. S.: Multiproxy evaluation of the Paleohydrology of the Sakarya River during the Last Milennium, NW Anatolia, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1067, https://doi.org/10.5194/egusphere-egu25-1067, 2025.

EGU25-1438 | Posters on site | SSP3.8

Climatic versus Anthropogenic Influences on Sediment Delivery to the Gulf of Mexico Marginal Sea since 5000 y BP 

Peter Clift, Bailey Wycoff, Andrew Carter, Samuel Mũnoz, and Tammy Rittenouer

We present a compilation of provenance data derived from the lower reaches of the Mississippi river showing how the source of sediment supplied to the lower reaches has changed through time in the recent geologic past. We integrate data from a late Holocene point bar, its associated oxbow lake (False River) and the channel plug that infilled since ~500 y BP, as well as another oxbow located upstream at Lake St John. Another finer grained sediment record was derived from coring close to the Mississippi south of New Orleans. The sediments were analysed for an array of major elements, Sr and Nd isotopes, as well as detrital zircon U-Pb geochronology. Grain size is a critical factor in controlling the provenance because suspended sediment is transported rapidly through the river compared to coarse-grained material which travels more slowly as bedload. The radiogenic isotope signature of the fine-grained sediment shows a long-term shift since 4.5 ka towards more radiogenic signatures indicative of more erosion from ancient continental crust, likely the Appalachians and Mid Continent rather than the Rocky Mountain foreland, although this remains the dominant source of material supplied to the Gulf of Mexico. While some of this shift may be anthropogenic, the trend suggests long-term drying of the continental interior and reduced erosion of the foreland. Nonetheless, sand-silt sized zircon U-Pb ages indicate that between 1600 and ~1920 CE flood sediments were dominated by supply from the Missouri River, which is largely sourced from the Rocky Mountain foreland. From 500 BCE until 1600 CE supply was more skewed to the Upper Mississippi and Red River, and with some input from the Arkansas River, also derived from the west. Coarse grained sediments deposited in the lower reaches during the last 10 years show a high degree of variability which we interpret to reflect reduced sediment buffering driven by the inability of the lower reaches to meander and recycle flood sediments in the way expected prior to the installation of levees. The modern tributaries all carry sediment that is much more altered than was true in the recent geological past and reflects heightened soil erosion driven by agriculture. The modern Mississippi is a poor analogue for the natural state of the river when compared to ancient geological deposits.

How to cite: Clift, P., Wycoff, B., Carter, A., Mũnoz, S., and Rittenouer, T.: Climatic versus Anthropogenic Influences on Sediment Delivery to the Gulf of Mexico Marginal Sea since 5000 y BP, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1438, https://doi.org/10.5194/egusphere-egu25-1438, 2025.

EGU25-1688 | ECS | Posters on site | SSP3.8

Sedimentary and diagenetic processes at the origin of the 3D architecture of heterogeneous lacustrine and palustrine limestones. 

Thibaut Jamey, Simon Andrieu, Céline Mallet, Gautier Laurent, Eglantine Husson, and Mohamed Azaroual

Lacustrine and palustrine carbonates form in lakes and swamps of various shapes and sizes. They can accumulate through chemical or biological processes and are constantly under the influence of external alteration sources such as meteoric waters, vegetation or fauna. Thus, there are the result of a complex primary fabric later modified by early and late diagenesis processes which makes them highly heterogeneous.

Their study is mainly motivated by their ability to act as a reservoir for underground water or for Carbon Capture & Storage (CCS), which both require a precise understanding of their structure and variability of permeable bodies.

The 3D architecture and the scale of heterogeneity of such carbonates remains a question as depositional and alteration processes can occur on centimetre scales or less (e.g., roots), to metre and kilometre scale (e.g., subaerial exposure). This variability cannot be assessed without any large, pluri-directional outcrop or without a high density of cored boreholes.

The O-ZNS platform (“Observatoire des transferts dans la Zone Non-Saturée”) located near Orleans, France, is an observatory of the vadose zone of the Beauce aquifer. The host rocks are aquitanian lacustrine and palustrine limestones (the Beauce Limestones formation).

The observatory offers an exceptional 20 m deep and 6 m diameter well surrounded by eight cored boreholes (20-25 m deep) within a radius of 30 m, which were described at a centimetric scale (1:6).

Our study focuses on the control of the 3D architecture of the sedimentary facies by understanding the chronology of the successive depositional environments. Also, it aims to consider the diagenetic overprint of the Beauce Limestones to decipher what is the impact of the primary fabric on secondary processes that finally lead to the heterogeneities we observe today.

This contribution will present: (1) How the 16 sedimentary facies distributed in 4 depositional environments (lake, lake margins, external palustrine, internal palustrine) vary at a decametric scale, (2) the paleo-environmental evolution of the site, located at the transition between lacustrine and palustrine settings, built thanks to the correlation of 8 transgressive-regressive cycles, and (3) the link between sedimentary facies, diagenesis and petrophysical properties (porosity, permeability).

How to cite: Jamey, T., Andrieu, S., Mallet, C., Laurent, G., Husson, E., and Azaroual, M.: Sedimentary and diagenetic processes at the origin of the 3D architecture of heterogeneous lacustrine and palustrine limestones., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1688, https://doi.org/10.5194/egusphere-egu25-1688, 2025.

International Ocean Discovery Program (IODP) Site U1417, located in the Surveyor Fan (Gulf of Alaska), preserves hemi-pelagic sediments influenced by glacial and fluvi­al depositional processes from the Cordilleran Ice Sheet in the Chugach–St. Elias Mountains and Coastal Mountains. A total of 441 samples from the late Miocene to early Pleistocene were used to measure the biogenic opal content and calculate its flux to trace the degree of diatom productivity in surface water and depositional history. In general, the biogenic opal content confirms the division of the lithostratigraphic units and subunits: diatom-bearing clay-rich intervals versus clast-rich terrigenous intervals. Despite large fluctuations from the late Miocene to early Pleistocene, the variation of biogenic opal content and deposition of biogenic opal flux might have been controlled by global climate change, such as the high levels during the Late Miocene Biogenic Bloom (LMBB) and mid-Pliocene Warmth (MPW) and its abrupt decline at the Northern Hemisphere Glaciation (NHG). These variations of surface water productivity may be attributed to the basin-to-basin redistribution of nutrients by global thermohaline circulation and the related Pacific Ocean ventilation in response to global climate change.

How to cite: Khim, B.-K., Kim, S., and Asahi, H.: Biogenic opal deposition in the Surveyor Fan (IODP Site U1417) of the North Pacific during the late Miocene to early Pleistocene, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1739, https://doi.org/10.5194/egusphere-egu25-1739, 2025.

East Asian summer monsoon (EASM) played key role in controlling the hydroclimate of East Asia continent regions. However, the Late Holocene changes of EASM in its northern margins are still unclear, which urgently needs to be revealed in the field of climate research. Here we systematically analyze the grain size of peat ash from core ZB-7 in the Zhibian peatland and core DFHN-2 in the Dongfanghongnan peatland to address this issue. Results show that the silt fraction occupies the most component of peat ash in cores ZB-7 and DFHN-2. The grain size distribution curves of peat ash of two cores display single peak pattern. The probability cumulative curves of two cores exhibit as two-sections mode. Three end-members (EMs) displaying single peak are identified in cores ZB-7 and DFHN-2. The EM2 of core ZB-7 and EM1 of core DFHN-2 represent the contributions of surface runoff. The EM2 of core ZB-7 demonstrates a series of periodicities, such as 1000a, 500a, 210a, 110a, 88a and 66a during the Late Holocene. The correlation relationship analyses indicate that the EM2 of core ZB-7 and total solar insolation (TSI) show opposite phase with El Niño-Southern Oscillation (ENSO) activities. Furthermore, five evolutionary stages of the EASM in northern margins were identified. Less ENSO activities and declined TSI regulated the decreased precipitation during stage 1 (4338-3479 cal. yr BP). The frequent ENSO activities and declined TSI induced low precipitation in stage 2 (3479-2297 cal. yr BP). In stage 3 (2297-949 cal. yr BP), the continuously decreasing ENSO activities resulted in high precipitation. Frequent ENSO activities and low TSI induced low precipitation during stage 4 (949-231 cal. yr BP). While the increase in TSI and decrease in ENSO activities regulated increased precipitation during stage 5 (231 cal. yr BP-Present). This study would expand our predictions on the future hydroclimate changes in monsoon northern margins.

How to cite: Zhang, M.: Late Holocene variations and driving mechanisms of the East Asian summer monsoon in northern margins: Evidence from peat ash grain size, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2109, https://doi.org/10.5194/egusphere-egu25-2109, 2025.

EGU25-2703 | ECS | Orals | SSP3.8

Bedding-parallel fibrous calcite veins in Permian carbonate, central Thailand 

Tindikorn Kanta and Piyaphong Chenrai

Bedding-parallel fibrous calcite veins (BPCVs) are prevalent in sedimentary basins and typically formed in petroleum source rock. This study examines the development of BPCVs in the Permian carbonate of the Khao Khwang Formation in central Thailand using petrographic, geochemical, and isotopic investigations, as well as total organic carbon (TOC) evaluation. Five rock specimens, comprising ten veins and five host rocks, were examined. The findings indicate that BPCVs display cone-in-cone and beef structures, categorizing them as unitaxial veins. The geochemical analyses and stable isotope compositions indicate that local fluid sources derived from inorganic carbonates and diagenetic formation fluids in the microbial methanogenic zone. Oxygen isotope analysis indicates that vein development occurred at late diagenetic stage. In situ U-Pb dating reveals that fibrous calcite veins originated from the Early to Middle Permian. The development of BPCVs linked to petroleum source rock provides critical insights into the history of fluids and petroleum generation within sedimentary basins.

How to cite: Kanta, T. and Chenrai, P.: Bedding-parallel fibrous calcite veins in Permian carbonate, central Thailand, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2703, https://doi.org/10.5194/egusphere-egu25-2703, 2025.

EGU25-4791 | ECS | Posters on site | SSP3.8

Modern Sedimentary Mechanisms and Evolution of Extreme Event Layers Offshore Southwestern Taiwan 

Bo-Hong Wang and Chih-Chieh Su

Taiwan is located in the western Pacific typhoon corridor and the Pacific Ring of Fire, where typhoons and earthquakes frequently happen, making submarine geohazards prone to occur. As the second longest river in Taiwan, the annual sediment load of the Gaoping River averages approximately 35.61 million tons, making it the dominant contributor of terrestrial sediments offshore southwestern Taiwan. Su et al. (2018) pointed out that the sedimentation rate in most areas offshore southwestern Taiwan is less than 0.5 cm/year, and the upper continental slope in the northern part is relatively more stable compared to the southern part. Natural disasters significantly influence sediment distribution and sedimentation processes off the southwestern Taiwan. In 2005, Typhoon Haitang caused heavy rainfall, leading to the rapid transport of large amounts of suspended materials from the Gaoping River to the offshore area of southwestern Taiwan. Based on the radionuclides data published by Huh et al. (2009), a distinct Typhoon Haitang event layer can be observed, and the high-activity layer associated with the 1963 global fallout can also be identified. In this study, we intend to integrate the findings of Huh et al. (2009) regarding the application of radionuclides with 13 box core samples collected in 2023 from the same locations (the shelf and slope areas on the northern and southern sides of the Gaoping Canyon). We aim to utilize the multi-tracer approach and grain size distribution to assess modern sedimentary event records, sediment transport pathways, and potential disaster risks offshore southwestern Taiwan. Additionally, we plan to analyze the correlation of sedimentary sequences across different coring sites, as well as their temporal variations in sedimentary records at the same site. The current results indicate a positive correlation between sediment porosity and water depth. Grain size analysis shows that the median grain size and sorting decrease as water depth increases. The higher sand content observed on the northern shelf is due to northward coastal currents and overflow effects at the canyon head. Future research will focus on investigating hydrodynamic differences across various layers to better understand sedimentary dynamics over the past two decades. This study will further examine how bioturbation affects radioactive dating results, which will help to establish a more accurate chronological model for sedimentary records.

 

References

Chih-An Huh, Hui-Ling Lin, Saulwood Lin, Ya-Wen Huang, Modern     accumulation rates and a budget of sediment off the Gaoping (Kaoping) River, SW Taiwan: A tidal and flood dominated depositional environment around a submarine canyon, Journal of Marine Systems, Volume 76, Issue 4, 2009, Pages 405-416, ISSN 0924-7963, https://doi.org/10.1016/j.jmarsys.2007.07.009

Su, C.-C., S.-T. Hsu, H.-H. Hsu, J.-Y. Lin, and J.-J. Dong, 2018: Sedimentological characteristics and seafloor failure offshore SW Taiwan. Terr. Atmos. Ocean. Sci., 29, 65-76, doi: 10.3319/TAO.2017.06.21.01

How to cite: Wang, B.-H. and Su, C.-C.: Modern Sedimentary Mechanisms and Evolution of Extreme Event Layers Offshore Southwestern Taiwan, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4791, https://doi.org/10.5194/egusphere-egu25-4791, 2025.

EGU25-5284 | ECS | Posters on site | SSP3.8

Study on the long-term shoreline extraction and analysis method on the east coast of Korea using Python toolkit 

Ho-Jun Yoo, Tae-Soon Kang, Dong-Soo Hur, and Sung-Soon Yoon

  In recent years, with the development of computer vision analysis and the free release of satellite images, it has become possible to observe and evaluate coastal and shoreline changes through satellite images. However, the shorelines obtained by satellite detection are instantaneous at the time of satellite capture, and some correction processes are required to validate them with actual monitoring data and ensure their reliability.

  In this study, Landsat and Sentinel-2 satellite images, along with a Python toolkit, were used to analyze shoreline data over a 40-year period on the east coast of Korea. Validation was performed using national research monitoring data collected bi-quarterly over approximately 10 years for 9 sites. Data containing changes greater than the standard deviation and errors in the data itself were removed from the shoreline results. The accuracy of the shoreline data was corrected by comparing it with monitoring data and reflecting the conditions of offshore external forces.

  All of the shoreline changes over the past 40 years have shown a relatively stable change of less than 3m per year. However, there has been rapid continuous change over the past 10 years. This is likely due to recent coastal development, including direct and indirect impacts from artificial structures, nourishment effects, and natural erosion.

  Continuous collection and analysis of shoreline change data are necessary to ensure the stability and management of coastal buffer zones, including coastal hinterlands and sandy beaches, long-term equilibrium, and continuous shoreline changes caused by extreme typhoons, human impacts, and changes in artificial structures. Ensuring coastal resilience and stability through satellite data and analysis methods is crucial. We plan to detect continuous shoreline changes on both the east and west coasts of Korea. Furthermore, research will be needed on digital twin-based data display to ensure convenience for stakeholders and respond effectively to coastal erosion.

How to cite: Yoo, H.-J., Kang, T.-S., Hur, D.-S., and Yoon, S.-S.: Study on the long-term shoreline extraction and analysis method on the east coast of Korea using Python toolkit, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5284, https://doi.org/10.5194/egusphere-egu25-5284, 2025.

       The Dangerous Grounds, located along the southern margin of the South China Sea, has undergone substantial tectonic and paleogeographic changes during the Cenozoic, spanning three distinct evolutionary stages: continental rifting, breakup from South China and southward drift, and collision with Borneo. This study utilized a robust dataset comprising 67 seismic reflection profiles, complemented by drilling and dredging data, to quantitatively reconstruct the sedimentary filling history of the Dangerous Grounds. By correlating sediment budget outcomes with the spatial distribution characteristics of sediment thickness, we have gained valuable insights into the region’ s geological evolution.

       Our findings reveal a progressive increase in sediment budgets across the three tectonic stages, despite relatively stable sediment budgets during the southward drift stage associated with seafloor spreading. Spatial analysis of sediment distribution, as revealed by sediment isopath maps, shows a continued decrease in the north and expansion in the south and west, suggesting the influence of regional tectonic transitions and variations in paleogeographic environment. By integrating the temporal and spatial distribution of depocenters with drilling results and sediment provenance geochemical analyses, we provides a comprehensive regional perspective on the factors controlling sediment budget trends, including regional tectonic transitions, variations in paleogeographic environment (such as climate, sea level, and sedimentary facies, and the evolution of local river systems).

       The sedimentary inputs to the Dangerous Grounds have shifted over time, with Paleocene-Eocene sediments primarily originating from the north. From the Oligocene to the Early Miocene, northern sediment supply progressively declined, while inputs from the southwest, transported through river systems originating in the Indochina and Malay Peninsulas, gradually increased. Since the Mid-Miocene, the collision with Borneo has led to enhanced sediment supply from the south, with sediments predominantly accumulating along slope edges, channel outlets, and within the Nansha Trough.

How to cite: Wang, F. and Ding, W.: Impacts of Tectonic-Paleogeographic Transitions on Cenozoic Sedimentary Distribution in the Dangerous Grounds, South China Sea, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5567, https://doi.org/10.5194/egusphere-egu25-5567, 2025.

Grain-size of clastic sediment is generally considered to be the result mainly of physical processes active during transport and deposition (e.g. grain-size sorting by dimension/density, sediment by-pass); less importance is generally given to other factors, such as the parent rock lithology. In this work, we investigate the control exerted by the parent rock lithology on the grain-size of daughter sediments. Our approach combines fieldwork-based sediment characterization (in-situ grain-size measurements and petrographic analysis of pebbles > 2 cm), laboratory analyses (sieving, measurement and petrographic point counting at the microscope on grains < 2 cm) and geospatial statistics of the source area.

To do so, we selected as study site a sandy-gravelly bar of the Avisio River, located in Valle di Fassa (Dolomites, Italy) which is sourced by a relatively small catchment area made by very different parent rocks. This allows us to disregard the effect of sediment transport from the source to the sampled depositional site, i.e. to consider the analysed samples representative of the sediment produced at the source by the studied catchment. The lithologies exposed in the catchment area are mainly represented by (i) dolostones, (ii) mafic to intermediate volcanics and (iii) limestones and sandstones, which all outcrop in similar proportions. From the fluvial bar, we collected sand and gravel samples analysing their dimensional (pebble measurements and grain-sizes sieving) and compositional properties (rock identification and sedimentary petrography). We analysed both the overall grain-size and composition of the collected samples and the composition of each grain-size fraction between 16 cm and 0.075 mm contained in each sample. Moreover, we performed a GIS-based geospatial analysis of the sediments source area to quantify the rock type distribution and have the true geology of the source region to be compared with its image provided by its daughter sediments.

Our results show a significant relationship between grain-size and sediment composition: gravels are mainly made by dolostone pebbles, while sands are mainly composed of volcanic grains. This trend persists across the separated grain-size portions: sediment fractions > 1 mm are richer in dolostone grains, while sediments fractions < 1 mm are richer in volcanic grains, and proves that dolostone and volcanic rocks feed at the source daughter sediments with dramatically different grain-size curves. Moreover, none of the samples shows the same proportion of the compositional distribution derived from the GIS-based geospatial analysis (i.e., similar proportion between the three lithologies considered).

These findings indicate that since their origin, sediment grain-size is strongly controlled by different weathering effects on the diverse parent rocks and therefore distinct grain-sizes provide very different geologic scenarios for the same source rock geology. This, while often overlooked, significantly impact provenance studies aimed to paleo-geologic reconstructions and must be also carefully considered in facies tract models, challenging the assumption that grain-size variations along depositional systems are solely due to physical processes acting on sediments having at the origin a simple grain-size distribution.

How to cite: Pezzoli, S., Menegoni, N., and Di Giulio, A.: Parent rocks control on grain-size of daughter sediments and implications for provenance studies: insights from the Avisio River (Dolomites, Italy), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6440, https://doi.org/10.5194/egusphere-egu25-6440, 2025.

EGU25-6880 | Orals | SSP3.8

Ayeyarwady-Thanlwin Rivers Shelf Sediment Dispersal: A High-Discharge Tidally-Dominated Monsoon-Influenced Tectonically-Active Setting 

Steven Kuehl, Evan Flynn, Day Wa Aung, Ko Yi Hla, and Courtney Harris

The Ayeyarwady-Thanlwin rank among the world’s top three river systems in terms of sediment load, and discharge into the energetic shelf environment of the Northern Andaman Sea.  The fate of this material has been investigated through a range of interdisciplinary studies since a 2017 field campaign to the present, and here we synthesize the resulting findings based on a combination of sedimentological, geochemical and oceanographic insights.  With no dams along the mainstems, this system has remained in a relatively steady-state condition during the past century, despite increasing human pressure, primarily from land-use changes and river sand mining. Tectonic setting plays a first-order control on the fate of the rivers’ sediment, with the formation of a mid-shelf pull-apart basin, the Martaban Depression, that serves as the major depocenter for this system.  Oceanographic conditions conspire to feed the rivers’ sediment into the Depression through the action of tides, waves and monsoon-driven circulation.  Extreme tides up to 7 m in amplitude keep sediment in suspension in an extensive shallow embayment, the Gulf of Martaban, before this material is released to the offshore Depression, likely because of some combination of spring-neap excursions, near-bed turbidity flows, or rapid offshore transport during cyclones.  Monsoon winds drive circulation toward the east during the SW Monsoon, coincident with the period of highest river discharge, further focusing sediment discharged from the numerous western Ayeyarwady distributaries into the Gulf.  Modeling results suggest surface and bottom net transport toward the Gulf may occur throughout the year.

Seabed geochemistry contributes much toward our understanding of shelf circulation and sediment dispersal patterns, and the preservation of the immense sediment-associated terrestrial organic carbon discharged by the rivers.  Core-scanning XRF elemental ratios show pronounced east-west trends that are attributed to three distinct sources: the Ayeyarwady, Thanlwin, and small rivers draining the Indo-Burman Range (IBR).  Distinct geochemical signatures on the shelf fronting the IBR suggest that sediment dispersal from the Ayeyarwady-Thanlwin is largely constrained to the Andaman Sea shelf. Downcore profiles of stable carbon isotopes from the Northern Andaman Sea show remarkably uniform values during the past century, suggesting that land-use changes evident in the catchment, especially during the past 50 years, are not preserved in the offshore record.  We suggest that extensive tidal reworking in the Gulf efficiently mutes such signals in the downcore record. Organic carbon studies further suggest that very little remineralization of terrestrial organic matter occurs during transport from the Gulf to the Depression, despite reworking and consequent oxidation in the Gulf.  Based on geochemical budgets of particle-reactive radionuclides scavenged from seawater, we estimate that significant onshore flow of open ocean water must occur, along with the substantial input of marine organic matter.  The absence of an observed “sediment priming” effect reflets the recalcitrant nature of this carbon pool.  The Ayeyarwady-Thanlwin system represents an end member within the family of such systems, and underscores the role of tectonic and oceanographic conditions in determining sediment dispersal and accumulation patterns in the marine environment.

How to cite: Kuehl, S., Flynn, E., Wa Aung, D., Yi Hla, K., and Harris, C.: Ayeyarwady-Thanlwin Rivers Shelf Sediment Dispersal: A High-Discharge Tidally-Dominated Monsoon-Influenced Tectonically-Active Setting, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6880, https://doi.org/10.5194/egusphere-egu25-6880, 2025.

EGU25-7363 | Orals | SSP3.8

Continental input and its relationship with biological sedimentary constituents over the MIS 6 to MIS 1 in the SW Gulf of Mexico 

Elsa Arellano-Torres, Sandra M. Villafuerte-Bazaldua, Priyadarsi Roy, and Juan José Kasper-Zubillaga

To unveil the relationship between reconstructed paleoclimatic and paleoceanographic changes based on geochemical proxies, we analyzed the marine sediment Core RC10-265PC retrieved from the Gulf of Mexico (GoM). The core spans the interval from Marine Isotope Stage (MIS)-6 to MIS-1 at a glacial to interglacial scale resolution. We studied the relationship between changes in biogenic constituents as proxies of primary productivity and those in continental terrigenous contributions as a source of micronutrients. The core constituents were identified and described by determining carbon content, the elemental concentration by X-ray fluorescence (XRF), and the mineral phases by X-ray diffraction (XRD). The biological constituents include total organic carbon (TOC) and calcium carbonate (CaCO3), whereas terrigenous constituents mainly include the major elements Si, Fe, K, Al, and Ti. In the core, we observed four ash deposits with high Si, K, and Zr concentrations but low in Al, Fe and Ca. Although they were a few cm thick, they did not contribute to increasing primary production. The XRD analysis in the bulk sediments shows that the most abundant mineral phases are calcite, phyllosilicates, quartz, feldspar, and pyroxene. Overall, increases in terrigenous components occurred during the early MIS-6, from MIS-5e to MIS-2, and during MIS-1. In parallel, a decrease in CaCO3 occurred, sometimes coincident with TOC increases. The former suggests a dilution of calcareous by terrigenous components that possibly arrived at the basin by riverine inputs. Such an input increase is not in tune with the latitudinal displacement of the Intertropical Convergence Zone nor with orbital periodicities. However, neighbouring evidence suggests moisture and runoff increase at the regional level, revealing that the oligotrophic oceanographic conditions in the GoM have remained for approximately 180 ka. Such findings expose several ecological implications if eutrophic conditions emerge under modern climate change.

How to cite: Arellano-Torres, E., Villafuerte-Bazaldua, S. M., Roy, P., and Kasper-Zubillaga, J. J.: Continental input and its relationship with biological sedimentary constituents over the MIS 6 to MIS 1 in the SW Gulf of Mexico, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7363, https://doi.org/10.5194/egusphere-egu25-7363, 2025.

The Ayeyarwady and Thanlwin Rivers deliver ~485 Mt of sediment/year to the northern Andaman Sea. The Ayeyarwady river mouths empty via the Ayeyarwady Delta, while the Thanlwin empties into the Gulf of Martaban located east of the delta. The Gulf of Martaban is a macrotidal, shallow embayment, and the abundant sediment supply and tidal energy make it one the world’s largest perennially turbid zones. Seasonal monsoons bring high precipitation during summer when winds are energetic and from the southwest (SW), and dry during winter when winds are moderate and from the northeast (NE). Surface circulation implies that sediment would be trapped in the northern Andaman Sea during SW monsoon and exported to the Bay of Bengal during the NE monsoon. A clinoform depocenter has been found seaward of the Gulf, and a second depocenter on the northwest side of the delta in the Bay of Bengal. The phasing and timing of sediment delivery to these depocenters has relevance for sediment budget, event preservation, and carbon cycling, however, the sediment delivery mechanisms to these depocenters remain a question.

To address this, a coupled hydrodynamic and sediment transport numerical model was used to quantify suspended sediment dispersal offshore of the Ayeyarwady delta and within the Gulf of Martaban. Based on the Regional Ocean Modeling System (ROMS), it accounted for suspended sediment fluxes and used SWAN (Shallow Waves Nearshore) for waves. Open boundary and atmospheric conditions were derived from available global model products to account for larger scale ocean conditions and winds. The model has been run using different versions of initial sediment bed grain size distributions, based on either simple assumptions or historical and recent grain size observations. The magnitude of suspended sediment flux shows sensitivity to the initial grain size distribution, but the overall seasonal and tidal trends are less sensitive.

Model applications to date have focused on quantifying the variability of suspended sediment flux over tidal and seasonal timescales. The model has been run for two one-month cases: one each representative of the winter and the summer monsoon. Results indicated that offshore of the delta, surface currents flowed eastward during the summer monsoon and westward during the winter monsoon. The bottom currents offshore of the delta, however, showed less dependence on seasonal signals and were westward on average for both the summer and winter model runs. Within the macrotidal Gulf of Martaban, turbidity was maintained by asymmetric tidal trapping. Sediment export from the Gulf primarily directed toward the Martaban Depression Clinoform, with very little sediment delivered westward to the Bay of Bengal.  Sediment export was larger during the summer than the winter monsoon, and especially high during spring tides that extended the turbid area to the vicinity of the clinoform.  

How to cite: Harris, C. and Du, Z.: Seasonal and tidal variability in suspended sediment dispersal offshore of the Ayeyarwady delta, Myanmar: results from a numerical model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7518, https://doi.org/10.5194/egusphere-egu25-7518, 2025.

EGU25-7649 | Orals | SSP3.8

Sediment source to sink process and controlling mechanism from the Bengal Bay to the East Siberian Sea of Asian continental margin  

Xuefa Shi, Shuqing Qiao, Shengfa Liu, Jianjun Zou, Yanguang Liu, Zhengquan Yao, Kunshan Wang, Limin Hu, and Jingrui Li

The Asian continental margin is located at the convergence and collision boundary of the Eurasian, Pacific and Indo-Australian plates, and is subjected to the strongest land-sea interactions and the most frequent exchanges of material and energy. The rivers in the Asian continental margin contributes about two-thirds of the global sediments from rivers to the ocean, which has a great impact on the sedimentation, biogeochemical processes and marine ecology of the marginal seas and the global oceans. Through international cooperation, we have studied the sediment source to sink system and paleoenvironment in the Asian continental margin from the East Siberian shelf in the north to the Bay of Bengal in the south. We compiled a serial of sediment type map with different scales of the Asian continental margin, and elaborated the distribution pattern of the sediments; We established a set of effective provenance tracing index system to elucidate the properties of fluvial sediments, identified the sediments provenance in Bay of Bengal, east China seas, Sea of Japan, and East Siberian Sea, described the transport and deposition processes of the fluvial sediment in the sea, and established the sedimentation model for the key areas; The source, input mode and burial of organic carbon on the shelf at different latitudes and their response to natural processes and human activities have been quantitatively evaluated; The controlling mechanism of sediment source-sink process impacted by the Asian monsoon, sea level change, uplift of Tibetan Plateau, sea current and sea ice variations has been revealed.

How to cite: Shi, X., Qiao, S., Liu, S., Zou, J., Liu, Y., Yao, Z., Wang, K., Hu, L., and Li, J.: Sediment source to sink process and controlling mechanism from the Bengal Bay to the East Siberian Sea of Asian continental margin , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7649, https://doi.org/10.5194/egusphere-egu25-7649, 2025.

EGU25-8410 | ECS | Orals | SSP3.8 | Highlight

Sedimentary Signatures of Typhoon: Insight from Core Record in the South China Sea 

Yu-Huang Chen, Chih-Chieh Su, Pai-Sen Yu, Tai-Wei Hsu, Sheng-Ting Hsu, Hsing-Chien Juan, and Yuan-Pin Chang

Sedimentary records of event deposits are crucial for regional natural disaster risk assessments and hazard history reconstructions. This study aims to identify deep-sea typhoon deposits through immediate post-event sampling following super typhoon Haiyan (2013) and typhoon Morakot (2009). After super typhoon Haiyan passed through the South China Sea in 2013, five gravity cores were collected along the typhoon path in the southern South China Sea Basin (>3800 mbsl). The results showed that Super Typhoon Haiyan deposits with clear graded bedding are preserved at the top of all cores. The thickness of the typhoon layers ranges from 20 to 240 cm and is related to changes in typhoon intensity. The lack of river-connected submarine canyon systems limited the transportation of terrestrial sediments from land to sea. Super Typhoon Haiyan-induced large surface waves played an important role in carrying suspended sediment from the Philippines. A distinctive feature is that Mn-rich layers were found at the bottom of the typhoon layers, potentially linked to the soil and rock composition of the Palawan region, which experienced tsunami-like storm surges caused by super typhoon Haiyan. Similar Mn-rich layer characteristics were also observed in the typhoon Morakot (2009) layer in the sediment cores from the lower reach of Gaoping submarine canyon. These Mn-rich layers may serve as a proxy for sediment export from large-scale extreme terrigenous events. This study provides the first sedimentary record of extreme typhoon events in the deep basin of South China Sea, which may shed light on reconstructing regional hazard history.

How to cite: Chen, Y.-H., Su, C.-C., Yu, P.-S., Hsu, T.-W., Hsu, S.-T., Juan, H.-C., and Chang, Y.-P.: Sedimentary Signatures of Typhoon: Insight from Core Record in the South China Sea, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8410, https://doi.org/10.5194/egusphere-egu25-8410, 2025.

EGU25-8426 | ECS | Orals | SSP3.8

Relative influence of allogenic forcings on shallow-marine sedimentary archives, Taiwan Western Foreland Basin 

Amy I. Hsieh, Romain Vaucher, James A. MacEachern, Christian Zeeden, Chuqiao Huang, Andrew T. Lin, Ludvig Löwemark, and Shahin E. Dashtgard

An analysis of allogenic forcing on shallow-marine strata of the Miocene–Pliocene Kueichulin Formation in the Taiwan Western Foreland Basin shows that changes in the sedimentary record were predominantly driven by: 1) orogenesis and basin subsidence, 2) precession-driven changes in hydroclimate, and 3) obliquity-driven changes in atmospheric and ocean circulation.

The transition from a wave-dominated open shelf to a tide-dominated shallow-marine deltaic environment was influenced by a combination of basin subsidence and the denudation of Taiwan. The rapid deepening of the Western Foreland Basin near 5400 Ka and low sedimentation rates resulted in the formation of lower offshore to distal delta front environments, characterized by limited fluvial and storm influences. Shallow-marine deltaic environments formed as sediment from Taiwan filled the Western Foreland Basin, as a result of accelerated uplift after 4920 Ka, and rapid erosion of the orogen by tropical cyclone precipitation intensified. Tidal currents also intensified as the paleo-Taiwan Strait became shallower and narrower with continued uplift and southwest migration of Taiwan. The sedimentary record also shows a strong link between sedimentation and hydroclimate, driven by eccentricity-modulated precession. Tropical cyclone deposition corresponds to precession maxima, with amalgamated beds that form during periods of sea-level minima. Periods of high obliquity and associated changes in atmospheric and ocean circulation also resulted in a strengthening of tidal currents, recorded as a prevalence of tidal beds in the stratal record.

The findings of this study demonstrate the effectiveness of shallow-marine strata as a paleoenvironmental archive with the potential to resolve the influence of competing allogenic controls on sedimentary systems, which is crucial for understanding how depositional systems responded to climate change, tectonic activity, and sea-level fluctuations throughout Earth’s history.

How to cite: Hsieh, A. I., Vaucher, R., MacEachern, J. A., Zeeden, C., Huang, C., Lin, A. T., Löwemark, L., and Dashtgard, S. E.: Relative influence of allogenic forcings on shallow-marine sedimentary archives, Taiwan Western Foreland Basin, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8426, https://doi.org/10.5194/egusphere-egu25-8426, 2025.

EGU25-8616 | ECS | Orals | SSP3.8

Controls on sedimentary deposits in the coastal environments of the Paris Basin at the Eocene-Oligocene transition. 

Mathilde Beernaert, Laurence Le Callonnec, Fabrice Minoletti, Hugues Bauer, Didier Merle, Jean-Paul Baut, and Bertrand Génault

The Eocene-Oligocene Transition (‘EOT’) marks a global deterioration in climate associated with the establishment of the Antarctic polar ice cap, but is poorly constrained in continental areas. In Europe, a marked seasonality and a major replacement of European flora and fauna by Asian species (the ‘Grande Coupure’ described by Stehlin, 1909) were recorded during this period. Deposits at the ocean-continent interface are recorded in the Paris Basin at the EOT, from the lagoon-marine to the lacustrine domains. Lithology and facies distribution are therefore controlled by mechanisms on a global and local scale (tectono and glacio-eustatism, climate, tectonic), which need to be differentiated and highlighted. We present a mineralogical, elemental and isotopic geochemistry record of three Upper Priabonian to Upper Rupelian sections located in the northern Paris basin (Cormeilles-en-Parisis, Le Pin-Villeparisis and Saint-Soupplets), near the Bray anticline. Cormeilles-en-Parisis, the westernmost, is located in the Saint-Denis synclinal and shows the most complete sedimentary sequence, more clayey and carbonaceous. It is fossiliferous but not very diverse. The Saint-Soupplets section, located on the eastern flank of the perianticlinal end of the Bray, shows the same sequence of formations as the Cormeilles-en-Parisis section, but is characterised by sandier deposits with current and erosive figures. The Le Pin-Villeparisis section, located on the western flank of the Bray anticline and between the two other sections, is truncated in its upper part and relatively condensed. It is essentially clayey and mostly barren of fossils.

In the Upper Priabonian, the sedimentary record shows a tectonic pulse at the origin of terrigenous inputs and the creation of positive topography, then the Late Eocene regression and the decrease of the tectonic activity inducing the progradation of continental deposits. In the Lower Rupelian, the long-term increase in detrital terrigenous deposits and the environmental changes suggested by floral and faunal data are probably due to the combination of tectonics and eustatism. To the west (Cormeilles-en-Parisis section), a few evaporitic levels show a lagoonal environment that is almost always submerged. To the east, the sections are incomplete (erosive levels and missing formations), influenced by the structure of the anticline, which forms a topographic barrier and a positive relief. The absence of certain formations and the presence of a clearly lacustrine formation at the top of the Le Pin-Villeparisis section show the proximity of the coastline, which is more prone to emersion when subjected to tectonic uplift. 

 

Reference: 

Stehlin, H., 1909. Remarque sur les faunules de mammifères des couches éocènes et oligocènes du Bassin de Paris. Bull. Société Géologique Fr. 19, 488–520.

How to cite: Beernaert, M., Le Callonnec, L., Minoletti, F., Bauer, H., Merle, D., Baut, J.-P., and Génault, B.: Controls on sedimentary deposits in the coastal environments of the Paris Basin at the Eocene-Oligocene transition., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8616, https://doi.org/10.5194/egusphere-egu25-8616, 2025.

EGU25-9213 | Orals | SSP3.8

Interstitial soluble salts in Dead Sea lakes sediments as monitors of the East Mediterranean-Levant hydroclimate during the past ~ 100 kyr 

Mordechai Stein, Omri Khalifa, Pamela Schimmer, Amitai Katz, and Boaz Lazar

Temporal variations in the Na/Cl, Mg/Cl, Br/Cl, Br/Mg ratios of deep brines that filled the Dead Sea Basin during the past ~100 kyr were retrieved from soluble salts within the lake’s sediments. The soluble salts were extracted from cores drilled in the Dead Sea floor and sediments of the last glacial from the high margins of the Dead Sea. The variations in these elemental ratios (e.g., declining/rising Na/Cl ratios) reflect processes of halite precipitation/dissolution during arid/wet periods in the drainage basin, respectively, and exchanges between the epilimnion and hypolimnion brine. Ions of Na+ and Cl- were mainly supplied to the brines by the dissolution of the Mount Sedom salt diapir and halite deposits at the lake’s margins (e.g., halite which precipitated during arid periods of the last interglacial). The main observations are: (1) Between ~100-30 ka the deep lake’s hypolimnion evolved through a steady “enrichment” by Na+ and Cl- ions, due to continuous dissolution of marginal halite and/or from the Mt. Sedom salt diapir. Towards the end of this period, between ~43-30 ka, the Amiaz plain, a marginal basin, that comprised a semi-isolated water body, witnessed frequent episodes of halite precipitation/dissolution with temporal patterns that resemble millennial temperature (δ18O) variations in the Greenland ice core; (2) Between ~30-18 ka (MIS 2), when Lake Lisan reached its highest stands and maximum spatial expansion, the soluble salts indicate on frequent changes in the composition of the hypolimnion, reflecting centennial dissolution cycles of the Mt. Sedom salt diapir; (3) Between ~18-9 ka, when the lake declined to low levels, the variations in the elemental ratios reveal several episodes of enhanced supply of freshwater to the shrinking lake, causing massive halite dissolution and supply of Na+ and Cl- to the hypolimnion. The long-term (~100 kyr) pattern in the elemental ratios of the hypolimnion resembles global CO2 concentrations and sea temperature trends, while the short-term fluctuations in these ratios are correlated with short warm/cold cycles in the Greenland ice core δ18O data, indicating a strong impact of the global climate engines on the regional hydro-climate in long and short time scales.

How to cite: Stein, M., Khalifa, O., Schimmer, P., Katz, A., and Lazar, B.: Interstitial soluble salts in Dead Sea lakes sediments as monitors of the East Mediterranean-Levant hydroclimate during the past ~ 100 kyr, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9213, https://doi.org/10.5194/egusphere-egu25-9213, 2025.

EGU25-9273 | ECS | Orals | SSP3.8

Elementome trajectories: a framework for studying ecosystem biogeochemical shifts in paleoenvironmental records. 

Javier de la Casa Sánchez, Josep Peñuelas, Miquel de Cáceres, Jordi Sardans, Sergi Pla-Rabés, Mario Benavente, Santiago Giralt, Armand Hernández, Pedro Raposeiro, Álvaro Castilla-Beltrán, Lea de Nascimento, and Sandra Nogué

X-ray fluorescence (XRF) and other advanced analytical techniques provide detailed information on geochemical composition in chronologically dated sedimentary sequences. These methods yield high-resolution data on elemental concentrations and ratios, enabling the reconstruction of past environmental conditions. In this contribution, we introduce a novel approach that uses multivariate analysis of all available biogeochemical and geochemical data (elementome) to characterize the trajectories of elemental composition over time and link them to drivers of environmental change. Our analysis of records from Atlantic islands, characterizing the magnitude, graduality and direction of biogeochemical shifts in paleoecological records from several archipelagos, shed light to a potential modern-time shift towards organic-dominated elementomes; and on the effect of human arrival and climate changes on the stability of ecosystem elementomes. Moving ahead, elementome trajectories hold promise as descriptive tools for paleoecology, but also in the interpretation of biogeochemical shifts at any timescale.

How to cite: de la Casa Sánchez, J., Peñuelas, J., de Cáceres, M., Sardans, J., Pla-Rabés, S., Benavente, M., Giralt, S., Hernández, A., Raposeiro, P., Castilla-Beltrán, Á., de Nascimento, L., and Nogué, S.: Elementome trajectories: a framework for studying ecosystem biogeochemical shifts in paleoenvironmental records., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9273, https://doi.org/10.5194/egusphere-egu25-9273, 2025.

EGU25-9382 | ECS | Orals | SSP3.8

Sediment recycling in the South Pyrenean Foreland Basin: impact of grain size and source rock distribution on compositional signatures 

Marta Roigé, David Gómez-Gras, Xavier Coll, Daniel Stockli, Antonio Teixell, Salvador Boya, and Miquel Poyatos-Moré

Sedimentary provenance studies have long played a crucial role in elucidating source-to-sink processes across various tectonic settings throughout geological time. Foreland basins, in particular, record the erosional and exhumation history of their source areas, offering valuable insights into the chronology of deformation and the evolution of drainage areas. However, detrital signatures do not always fairly represent the composition of their drainage areas. Therefore, efforts are needed to better understand the factors controlling signal propagation from primary sources to ultimate sinks. The Jaca-Pamplona basin in the southern Pyrenees provides an excellent opportunity to explore the propagation and distribution of provenance signals in a setting with multiple source areas. We present combined data from detrital zircon U-Pb dating, sandstone petrography, and pebble point counting which allow us to infer the source area composition, its evolution, and the controls on provenance signal propagation. Our results indicate that alluvial fans had a source area composed of the North Pyrenean Zone and earlier, deep-marine synorogenic deposits, as evidenced by the overwhelming presence of recycled turbidite clasts. However, detrital zircon U-Pb age data from these alluvial fan deposits show a dominant Cadomian signature, while the turbidites exhibit a dominant Variscan signature, highlighting the complexity introduced by sediment recycling. We propose that the areal distribution of source rocks in the drainage area, transport distance, and differential weathering processes can explain this compositional effect. This is further supported by the clear grain-size dependence of the petrographic detrital modes, which show a positive correlation between grain size and the amount of recycled grains. Therefore, this study underscores the importance of integrating various provenance techniques to improve provenance reconstructions and to identify the intrinsic factors controlling the propagation and representativity of sediment sources.

How to cite: Roigé, M., Gómez-Gras, D., Coll, X., Stockli, D., Teixell, A., Boya, S., and Poyatos-Moré, M.: Sediment recycling in the South Pyrenean Foreland Basin: impact of grain size and source rock distribution on compositional signatures, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9382, https://doi.org/10.5194/egusphere-egu25-9382, 2025.

EGU25-9822 | ECS | Posters on site | SSP3.8

A multi-proxy reconstruction of past erosion dynamics based on lake sediments from the northern Ecuadorian Andes 

Bjarne Heyer, Lisa Feist, Volker Karius, Agnieszka Halaś, Michal Słowiński, Liseth Pérez, Patricia Mothes, Elizabeth Velarde-Cruz, Alejandra Valdés-Uribe, Ana Mariscal Chávez, and Elisabeth Dietze

Lake sediments in mountain areas worldwide have been analysed to reconstruct erosion dynamics on local to regional scales. In the tropical Andes, an area of globally-relevant biodiversity hotspots and carbon sinks, long-term erosion patterns in response to climate and land use change are poorly known. In this study we examine the local erosion history as archived in a high-elevation (<3,700m asl) caldera lake north of Ecuador’s capital Quito. A multi-proxy approach was conducted on a 72 cm-long lake sediment core retrieved from Caricocha in the Mojanda Lake Region, including visual core description, X-ray fluorescence (XRF) core-scanning, magnetic susceptibility (MS), C/N and grain-size analyses. Two radiocarbon dates were combined with tephra-stratigraphy to derive a viable timeframe for sediment accumulation. Data obtained from XRF, MS, C/N and grain-size analyses were evaluated using multivariate statistical methods. Results from cluster and principal component analysis revealed at least 3 stratigraphic units alternating with at least 8 tephra layers. We will discuss a multi-proxy approach to identify different sedimentary environments, sources of material and underlying patterns in this volcanically active region. Including log-transformed element ratios of the XRF data we report on the challenges to disentangle proxies for past erosion dynamics from further palaeoenvironmental conditions, of relevance for future land use under climate change.

How to cite: Heyer, B., Feist, L., Karius, V., Halaś, A., Słowiński, M., Pérez, L., Mothes, P., Velarde-Cruz, E., Valdés-Uribe, A., Mariscal Chávez, A., and Dietze, E.: A multi-proxy reconstruction of past erosion dynamics based on lake sediments from the northern Ecuadorian Andes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9822, https://doi.org/10.5194/egusphere-egu25-9822, 2025.

EGU25-11379 | ECS | Posters on site | SSP3.8

Superposition and Intra-Stratal Bedding: Comparing the effects of different diagenetic models on stratigraphy. 

Theresa Nohl, Axel Munnecke, and V. Paul Wright

The principles of stratigraphy, rooted in the foundational works of Nicolaus Steno, William Smith, and Johannes Walther, assert that sedimentary layers are deposited sequentially and preserve a temporal and environmental record. While these principles have guided stratigraphic interpretation for centuries, carbonate successions challenge their straightforward application due to the impact of diagenetic processes. This was clear to earlier work on diagenetic bedding by e.g. Robin Bathurst or Werner Ricken, who discussed the implications for their models. More recent work on early diagenetic transformations, including dissolution, cementation, and differential compaction, can modify or completely obscure primary depositional features, resulting as well in a specific type of secondary “diagenetic bedding,” introducing intra-stratal lithological patterns that mimic primary bedding but are unrelated to depositional events.

Here we compare the mechanisms behind a variety of types of diagenetic bedding, with a focus on their implications for stratigraphy, paleoenvironmental reconstruction, and geochronology. We demonstrate how secondary features can disrupt traditional stratigraphic assumptions, obscure temporal resolution by combining distinct depositional layers into single beds or splitting original layers into multiple diagenetic units, and explore how differential preservation of aragonitic and calcitic components introduces spatial and temporal variability in fossil records, potentially disrupting correlations across stratigraphic sections. We summarise for the individual diagenetic models the key features to identify diagenetic bedding and the potential implications for stratigraphic applications.

How to cite: Nohl, T., Munnecke, A., and Wright, V. P.: Superposition and Intra-Stratal Bedding: Comparing the effects of different diagenetic models on stratigraphy., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11379, https://doi.org/10.5194/egusphere-egu25-11379, 2025.

EGU25-11785 | Posters on site | SSP3.8

Facies modeling of Cenozoic successions in the Gunsan Basin using statistical methods 

Changyoon Lee and Sun Young Park

The Gunsan Basin is located between the eastern Chinese coast and the Korean Peninsula. The basin originated during the Cretaceous due to tectonic activity. After several rifting events, the final rift occurred during the Oligocene. Since the Miocene, the postrift phase has been ongoing to the present day. This study focuses on the interval of the final rifting event of the Cenozoic. The Gunsan Basin remains a frontier basin for hydrocarbon exploration, with only five wells drilled between 1975 and 1991. The study area is located in the eastern sag, known as the East Subbasin, approximately 26 km from the nearest well. Typically, more than 10 wells are needed near a reservoir to predict sand bodies effectively. In this study, we employed geostatistics to generate facies models. The Sequential Indicator Simulation (SIS), one of the stochastic methods, is particularly effective for modeling facies in areas with sparse well data. The pixel-based SIS approach is using trend maps, especially when lateral information is unavailable. These trend maps, derived from the RMS (Root Mean Square) attribute, are based on amplitude and help delineate facies. During the Miocene, the paleoenvironments in the depocenter and margin were lacustrine and littoral, respectively, and the lithology was interpreted as mudstone and sandstone. The transition from littoral to lacustrine environments is attributed to thermal subsidence. Through attribute analysis, we indirectly infer the rift system and the associated facies changes.

How to cite: Lee, C. and Park, S. Y.: Facies modeling of Cenozoic successions in the Gunsan Basin using statistical methods, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11785, https://doi.org/10.5194/egusphere-egu25-11785, 2025.

EGU25-11902 | ECS | Orals | SSP3.8

Spatial and temporal evolution of tidal channels' submarine geomorphology in the northern Venice Lagoon, Italy 

Taha Lahami, Irene Guarneri, Daphnie Galvez, Antonio Petrizzo, Mariacristina Prampolini, Valentina Grande, Giorgio Castellan, Federica Rizzetto, Federica Foglini, and Fantina Madricardo

Tidal environments are highly dynamic systems whose evolution is shaped by a complex interplay of natural and anthropogenic factors. These systems respond to intricate hydrodynamic processes such as tidal asymmetry, sedimentation, and channel morphodynamics. These environments are characterised by the presence of tidal channels, which are critical for ecosystem functioning as they facilitate the exchange of water, sediments, and nutrients. Despite their importance, the spatial and temporal evolution of tidal channels remains insufficiently studied, particularly in terms of their morphological and sedimentological characteristics. Information on their evolution is particularly relevant in densely populated areas, where natural processes are closely connected with anthropogenic pressures.

This study aims to explore the tidal channel seafloor characteristics and spatiotemporal evolution focussing on a case study from the northern Venice Lagoon.

With this aim, high-resolution MultiBeam Echo-Sounder (MBES) bathymetry and backscatter data were acquired over an eight-year period, in 2013 and 2021. Ground truth sediment samples and seabed video footage were collected to characterize the substrate and validate the maps produced from the MBES acoustic data. Morphological features were analyzed in a GIS environment using bathymetric data.  The analysis identified both erosional and depositional features, finding depositional features dominating the study area. A seafloor sediment map was generated by classifying backscatter data using the unsupervised Jenks Natural Breaks algorithm. To assess changes over time, data from 2013 were compared to those gathered in 2021. Our findings suggest that deposition processes were predominant, with an overall net sediment accumulation of 542.7 · 10³ m³, strongly influenced by anthropogenic activity, related to the recent operation of mobile barriers at the lagoon inlets and salt marsh restauration efforts in the area.

In the context of rising mean sea levels and associated adaptation measures, this work not only enhances understanding of highly valuable and vulnerable transitional environments but also helps to assess the long-term impact of anthropogenic interventions.

Aknowledgements

This work was partially carried out within the Research Program Venezia 2021, with the contribution of the Provveditorato for the Public Works of Veneto, Trentino Alto Adige and Friuli Venezia Giulia, provided through the concessionary of State Consorzio Venezia Nuova and coordinated by CORILA. The authors acknowledge the facilities of the International Centre for Advanced Studies on River-Sea Systems DANUBIUS-RI (https://www.danubius-ri.eu/ ) in undertaking this research.

How to cite: Lahami, T., Guarneri, I., Galvez, D., Petrizzo, A., Prampolini, M., Grande, V., Castellan, G., Rizzetto, F., Foglini, F., and Madricardo, F.: Spatial and temporal evolution of tidal channels' submarine geomorphology in the northern Venice Lagoon, Italy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11902, https://doi.org/10.5194/egusphere-egu25-11902, 2025.

EGU25-11989 | ECS | Posters on site | SSP3.8

Tephrochronological analysis of the Plio-Pleistocene Chemeron Formation, Baringo Basin, Kenya: Refining stratigraphy and constraining chronology of vertebrate fossil sites 

Adeera Batlay, Catherine Beck, John Kingston, Emma Mbua, Matthew M. Skinner, Tracy Kivell, and Habiba Chirchir

Tephrochronology provides a stratigraphic approach to correlating geologic and paleoenvironmental events using volcanic ash layers. Stratigraphic correlation, especially over local and regional scales, plays a vital role in tracing the evolutionary trajectory of our hominin relatives across space and time in eastern Africa. The goal of this study is to employ tephrochronology to distinguish tephra layers within the Chemeron Formation at the site of Sinibo, Kenya. The Chemeron Formation is a sequence of Plio-Pleistocene sediments spanning the 5.3 to 1.6 Ma interval in the eastern foothills of the Tugen Hills — a fault block in the Baringo Basin of the Kenyan Rift Valley. This formation is an ideal site for the application of tephrochronology, as it comprises multiple tuff units interbedded with fluvial and lacustrine deposits that yield mammalian fossils, including hominins. In this project tephra layers from the Sinibo section are differentiated by analysing the geochemistry of volcanic glass shards from the tephra and establishing potential isochronous volcanic events in the stratigraphic record. Tephra samples analysed in this study were collected in the field and analysed for major element geochemistry using an Electron Microprobe. Distinct tephras were reconfirmed, including the Lokochot and Tulu Bor tuffs that are found broadly across eastern Africa. Ultimately, the tephra sequence from the relatively continuous section at Sinibo will be used to constrain the chronostratigraphy of fossil sites in structurally disrupted sequences in the Chemeron Formation. This work builds upon previous analyses (Namwamba, 1993) and is integrated with existing stratigraphy.

How to cite: Batlay, A., Beck, C., Kingston, J., Mbua, E., Skinner, M. M., Kivell, T., and Chirchir, H.: Tephrochronological analysis of the Plio-Pleistocene Chemeron Formation, Baringo Basin, Kenya: Refining stratigraphy and constraining chronology of vertebrate fossil sites, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11989, https://doi.org/10.5194/egusphere-egu25-11989, 2025.

The relationship between depositional environments and transportation processes associated with the general properties of formed siliciclastic sediments has greatly interested researchers. The grain shape properties of the sediments reflect the transport mechanisms of different geomorphological and sedimentary environments. The spread of new, high-resolution analytical methods has made it possible to quickly examine the grain shape properties of a large number of individual mineral grains. We investigated three sediment types from different environments (aeolian, fluvial, glacial, [n=27]) using automated image analysis (Malvern Morphologi G3-ID). During the analysis and data processing (e.g. Kruskal-Wallis, MANOVA, PCA) we examined four variables related to grain shape, which were the following: HS circularity (form, roundness), convexity (surface texture), solidity (roundness) and elongation (form). Our vital aim was to determine the key variables that can help to distinguish certain geomorphological environments and define the possible limits and boundaries of each granulometric feature of the medium sand fraction (250-500 µm). Five groups were distinguished according to the three types of environment (p<0.001; α=0.05). The grains from the aeolian and glacial sediments each formed a separate group, while the grains from the fluvial environments were classified into three groups. HS circularity was the most effective attribute, and the elongation variable proved to be the least influential parameter in differentiating sedimentary environments. However, the high values (mean: 0.24-0.3) of the elongation variable indicate a very fresh state of grains from glacial and certain fluvial samples. The HS circularity value changes slowly over time, and a large amount of energy is needed to increase the roundness value, but relatively less time and presumably shorter distance are required to decrease the surface roughness. We tried to interpret the results by comparing the granulometric properties of recent sediment grains with paleo sediments (aeolian and fluvial, n=15). One additional group was formed containing the highest granulometric values of the investigated samples, and the other sediments were classified into the recent fluvial and aeolian groups. Although according to their stratigraphic position, they should have been classified into the opposite sediment groups, indicating that the paleo-aeolian sediments bear the transport features of the fluvial medium and vice versa. By increasing the number of samples and documentation of grains in various geomorphological environments makes it possible to delineate preliminary grain shape boundaries (e.g. for solidity glacial-fluvial: 0.95; fluvial-aeolian: 0.97). However, this may also have a hindering effect, as the grouping methods hide the differences in some parameters within the classified sediments. Presumably, for example, the aeolian environments may be as diverse as the fluvial ones and need to be studied separately. It is important to note that the presented granulometric fingerprinting method can only provide comprehensive and detailed insights into the depositional environment of the mineral particles when applied together with other proxies.

Support of the National Research, Development and Innovation Office (Hungary) under contract NKFIH FK138692 is gratefully acknowledged.

How to cite: Gresina, F., Farkas, B., Magyar, G., Szalai, Z., and Varga, G.: Comparison of recent sediments from different geomorphological environments using automated static image analysis with insight into its applicability to paleo archives, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12819, https://doi.org/10.5194/egusphere-egu25-12819, 2025.

Alum Shale is a finely laminated organic-rich sedimentary rock which has recorded an anoxic-euxinic period which lasted for more than 20 My during tthe Cambrian and early Ordovician in the current-day Scandinavian region. A younger section (Tremadocian) of Alum Shale formation is located in Estonia, eastern part of the Baltic Paleobasin.

A 10-meter section of Alum Shale (black shale) and associated sediments (glauconitic sandstone, grey shale, sandstone) were scanned in core PED-403 with a Geotek XRF analyser, attached to automated Geotek-MSCL workstation. The concentrations of Mo, U, Ti, Al, S, and Si were analysed and corrected by measuring in-house reference samples.

Mo and U mostly co-vary in the sediments, but certain sections indicate a preferential uptake of Mo instead of U, indicating periods where particulate shuttle was active during slightly more oxic periods. Fine laminae also contain very low Mo and U enrichments, pointing to short-lived oxygenated conditions instead of prevailing perennial oxygen minium zone conditions on the shelf. Suble redox changes do not correlate with sedimentary textures described in the core. Systematic cyclicity was detected in the case of Ti, Al and Si. Sørensen et. Al. (2020) have demonstrated that astronomically forced climate cycles have been recorded in Cambrian-age Scandinavian Alum Shale cores. With follow-up analyses we wish to reveal whether cycles detected in the Estonian core have similar forcings.

This study was supported by EGT-TWINN project (GA no 101079459).

How to cite: Vind, J., Plado, J., and Põldsaar, K.: Millimeter-scale scanning of redox-sensitive elements in Tremadocian Alum Shale for revealing subtle redox variations and cyclicity, northwestern Estonia, Baltic Palaeobasin, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13006, https://doi.org/10.5194/egusphere-egu25-13006, 2025.

EGU25-14906 | ECS | Posters on site | SSP3.8

Subsurface dissection of Holocene inter-reef Halimeda bioherms: morphology, facies and latitudinal variations in the northern Great Barrier Reef 

Zsanett Szilagyi, Luke Nothdurft, Jody Webster, Mardi McNeil, Juan Carlos Braga, Trevor Graham, Bethany C. Behrens, Yusuke Yokoyama, Robin Beamen, Victorien Paumard, Jeffrey Shragge, Sarah Goh, Jacquelin Reeves, Lara Picton, and Helen Bostock

Halimeda, calcareous green algae, bioherms are among the largest inter-reef biogenic structures in the Great Barrier Reef, spanning over >6000 km2 of the continental shelf – an area exceeding the adjacent coral reefs at equivalent latitudes1. Previous studies have shown the peculiar circular to reticulate shapes, the internal structure and volume of these accumulations, underscoring their significant contribution to the global neritic carbonate factory throughout the Holocene2,3. However, a comprehensive understanding of the formation and development of these uniquely shaped bioherms has been hindered by the absence of densely spaced core samples that target bioherm morphologies.

This study presents new data from the 2022 RV Investigator voyage IN2022_V07 “Halimeda bioherms: Origins, function and fate in the northern Great Barrier Reef (HALO)”. Forty-two densely spaced vibrocores were collected (up to 6 m length) over 3 inter-reef sites between lat 15⁰ 48’ 45” S and lat 13⁰ 21’ 11” S. Core locations to target bioherm morphotypes were collected with the aid of 50 cm resolution multibeam bathymetry data, and closely spaced sub-bottom profiles collected during the voyage. A total of almost 200 m of cores have been scanned with high-resolution CT, 50 m of core have been split, logged, scanned with multi-sensor core logger (magnetic susceptibility, spectrophotometer, X-ray fluorescence) and subsampled for grain size, composition and microfossil analysis to show a variety of facies ranging from estuarine to coral-rich deposits. Selected cores have been sub-sampled for radiocarbon dating of Halimeda grains, benthic foraminifers, and organic rich mud (23 samples), spanning from 12 ka to present, aligning with previous findings3. Initial observations revealed further facies complexity than previously thought in morphotypes, including Halimeda floatstone-rudstone and Foraminiferal wackestone-packstone facies in the south, while having facies minor mud matrix and richer in coral, mollusc, rhodolith and lithified clumps abundance towards north. This new dataset significantly advances our understanding of Halimeda bioherm morphology, development, and regional influences, providing new insights into their formation processes and ecological significance.

 

References:

  • McNeil, M. A., Webster, J. M., Beaman, R. J., and Graham, T. L., 2016, New constraints on the spatial distribution and morphology of the Halimeda bioherms of the Great Barrier Reef, Australia: Coral Reefs, v. 35, no. 4, p. 1343-1355. doi: 10.1007/s00338-016-1492-2
  • McNeil, M., Nothdurft, L. D., Dyriw, N. J., Webster, J. M., and Beaman, R. J., 2021, Morphotype differentiation in the Great Barrier Reef Halimeda bioherm carbonate factory: Internal architecture and surface geomorphometrics: The Depositional Record, v. 7, p. 176– 199. doi: https://doi.org/10.1002/dep2.122
  • McNeil, M., Nothdurft, L. D., Hua, Q., Webster, J. M., and Moss, P., 2022, Evolution of the inter-reef Halimeda carbonate factory in response to Holocene sea-level and environmental change in the Great Barrier Reef: Quaternary Science Reviews, v. 277. doi: 10.1016/j.quascirev.2021.107347

How to cite: Szilagyi, Z., Nothdurft, L., Webster, J., McNeil, M., Braga, J. C., Graham, T., Behrens, B. C., Yokoyama, Y., Beamen, R., Paumard, V., Shragge, J., Goh, S., Reeves, J., Picton, L., and Bostock, H.: Subsurface dissection of Holocene inter-reef Halimeda bioherms: morphology, facies and latitudinal variations in the northern Great Barrier Reef, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14906, https://doi.org/10.5194/egusphere-egu25-14906, 2025.

EGU25-15355 | ECS | Orals | SSP3.8

Luminescence dating of core DLC70-2 from the North Yellow Sea in China and its implication for late Quaternary transgressions 

Nan Tang, Zhongbo Wang, Penghui Lin, Yuexin Liu, Zonghui Wu, Haozheng Tian, Xi Mei, Jun Sun, Jianghao Qi, Rihui Li, Shuyu Wu, Hongxian Chu, and Zhongping Lai

Reliable chronology is crucial for reconstructing the sedimentary history and sea level fluctuations. However, the lack of robust ages for late Quaternary deposits on the North Yellow Sea (NYS) shelf hampered our understanding of its sedimentary processes. In this study, quartz optically stimulated luminescence (OSL) and feldspar post-infrared infrared stimulated luminescence (post-IR IRSL) dating protocol were utilized to establish a detailed chronostratigraphy for the upmost 30 m of core DLC70-2 from the central NYS. Based on lithology features and dating results, three transgressive layers (hereafter referred as T1, T2 and T3, respectively from top to bottom) were identified. The consistency between two OSL dates (10.3-6.7 ka) and six radiocarbon (14C) dates (10.4-4.9 cal ka BP) indicates that the T1 layer deposited during MIS 1. Five quartz samples yielded saturation ages of >53 ka, combined with one feldspar pIRIR290 age of 76±7 ka from the top of the T2, suggested that the T2 layer should have formed no later than MIS 5. For T3 layer, two saturated quartz ages of >71 ka and a feldspar corrected age (191±17 ka) revealed that the T3 layer has formed at least during MIS 7. 
Based on the renewed chronostratigraphy of core DLC70-2, we reconstruct a comprehensive late Quaternary stratigraphy using ten previously published cores from the Bohai Sea and Yellow Sea. The occurrence of cold-water species Buccella frigida and Protelphidium tuberculatum during MIS 5 indicates there existed a cold-water mass (cyclonic eddy) similar to present-day marine circulation. Additionally, the late Quaternary stratigraphic correlation is supported by the previously chronostratigraphic reconstruction of coastal loess. These findings will enhance our comprehending on the sedimentary processes and their paleo-environment changes on the eastern Chinese shelves during late Quaternary.
Key words: luminescence dating; North Yellow Sea; late Quaternary; stratigraphic construction; transgressive deposits; core DLC70-2

How to cite: Tang, N., Wang, Z., Lin, P., Liu, Y., Wu, Z., Tian, H., Mei, X., Sun, J., Qi, J., Li, R., Wu, S., Chu, H., and Lai, Z.: Luminescence dating of core DLC70-2 from the North Yellow Sea in China and its implication for late Quaternary transgressions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15355, https://doi.org/10.5194/egusphere-egu25-15355, 2025.

High-resolution (millennial-scale) chronology is becoming more and more important in sedimentary process reconstruction, which could uncover unexpected events, in particular hiatus. It is assumed that sediments in  endorheic basin should be continuous. However, Our large luminescence chronology data revealed that, since late Quaternary, hiatus were common in the cores of the endorheic Qaidam Basin in the Tibetan Plateau, especially in the Last Glaciation Maximum (LGM) during which the endorheic lakes dried up and then the wind erosion was dominant.

Our large dataset of luminescence dating in deltas/fluvial-plains also displayed similar discontinuous pattern in core sediments, demonstrating unexpected hiatus which was omitted by previous studies, as well as the impacts of human activities revealed by changes of sedimentation rate.

It is strongly recommended the wider application of high-resolution chronostratigraphic methods in sedimentary research, and dense sampling for optically stimulated luminescence (OSL) dating. The combination of Single Aliquot Regeneration (SAR) protocol (Murray and Wintle, 2003) and Standardized Growth Curve (SGC) protocol (Roberts and Duller, 2004; Lai, 2006), SAR-SGC (Lai and Ou, 2013), routine used in our laboratory, will be of great help in this regard, which could save machine measurement time for at least 70%.

Key words: Luminescence chronology; high resolution; hiatus; sedimentary process.

 

References

Lai, Z.P., 2006, Testing the use of an OSL standardized growth curve (SGC) for determination on quartz from the Chinese Loess Plateau: Radiation Measurements, 41, 9–16, doi:10.1016/j.radmeas.2005.06.031.

Lai, Z.P, Ou, X.J., 2013. Basic procedures of optically stimulated luminescence (OSL) dating. Progress in Geograpgy, 32, 683-693 (in Chinese with English abstract).

Murray, A.S., and Wintle, A.G., 2003, The single aliquot regenerative dose protocol: potential for improvements in reliability: Radiation Measurements, 37, 377–381, doi:10.1016/S1350-4487(03)00053-2.

Roberts, H.M., and Duller, G.A.T., 2004, Standardised growth curves for optical dating of sediment using multiple-grain aliquots: Radiation Measurements, 38, 241–252, doi:10.1016/j.radmeas.2003.10.001.

How to cite: Lai, Z.: Chronological data is the best proxy in sedimentary process reconstruction, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15450, https://doi.org/10.5194/egusphere-egu25-15450, 2025.

EGU25-15862 | Orals | SSP3.8

Submarine geomorphology of tidal channels in the northern Venice Lagoon, Italy 

Mariacristina Prampolini, Taha Lahami, Giorgio Castellan, Daphnie Galvez, Antonio Petrizzo, Valentina Grande, Christian Ferrarin, Federica Foglini, Federica Rizzetto, and Fantina Madricardo

The morphodynamics of coastal tidal wetlands and salt marshes are closely tied to the tidal channel networks that link these ecosystems to the sea. Tidal channels, shaped by strong currents and dynamic bathymetry, are vital for sediment transport and key ecological functions in coastal environments. They act as pathways for sediment, nutrients, and organic matter, supporting the health and resilience of tidal wetlands. These networks provide essential ecosystem services, including erosion control and habitats for fish and shellfish, which are crucial for biodiversity and fisheries.

However, tidal wetlands face growing threats from human activities. Dredging disrupts sediment transport and alters flow patterns, leading to habitat loss. Increased navigation accelerates bank erosion and raises water turbidity, degrading habitat quality. Coastal infrastructure, such as seawalls and dikes, further fragments these ecosystems, disrupting natural hydrological processes. Climate change exacerbates these pressures through rising sea levels and more frequent storms, accelerating wetland degradation.

Understanding the geomorphology and sediment dynamics of tidal channels is critical for managing these ecosystems, to mitigate natural and human-induced changes, enhance biodiversity, and promote sustainable management. Geomorphological studies often rely on satellite imagery and aerial surveys to analyze channel morphology and path changes. Seismic surveys and laboratory experiments contribute to understanding large-scale and fine-scale geomorphic processes. However, few studies employ high-resolution multibeam echosounder systems to document the detailed underwater morphology of tidal channels, with limited work on their three-dimensional structures.

This study aims to deliver a detailed 3D mapping of the seafloor morphology and sediment distribution in the tidal channels of the northern Venice Lagoon (Italy), one of the most studied coastal lagoons globally. While many studies have explored the migration and evolution of Venetian tidal channels, fewer have focused on high-resolution 3D mapping of their underwater features. We conducted morphometric analyses and classified channel substrates by means of high-resolution multibeam echosounder data validated with grab samples and video footage. The approach integrated bathymetric derivatives, expert geomorphic interpretation, and supervised classification of acoustic backscatter to produce a comprehensive understanding of tidal channel features.

The findings reveal fine-scale details of tidal channel seafloor geomorphology, providing new insights into their structure and functioning. This research enhances our understanding of tidal channel dynamics and offers valuable information for preserving and managing these critical ecosystems effectively.

How to cite: Prampolini, M., Lahami, T., Castellan, G., Galvez, D., Petrizzo, A., Grande, V., Ferrarin, C., Foglini, F., Rizzetto, F., and Madricardo, F.: Submarine geomorphology of tidal channels in the northern Venice Lagoon, Italy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15862, https://doi.org/10.5194/egusphere-egu25-15862, 2025.

EGU25-18440 | ECS | Posters on site | SSP3.8

A new sediment mobility and seabed disturbance geo-spatial toolbox (Sed-mob-bed Tool) 

Shauna Creane, Aelita Totska, and Mark Coughlan

On continental shelf seas, the spatial and temporal interaction between hydrodynamic processes and seabed substrate impacts seabed evolution and sediment distribution. For instance, when the magnitude of bed shear stress, induced by waves and/or currents, is greater than the threshold of movement, sediment is mobilised, giving rise to a range of dynamic bedforms and intricate local and regional sediment transport systems. These processes have direct implications for a wide range of offshore economic exploits (e.g., siting renewable energy and telecommunication infrastructure).

This area of research is currently at the forefront of policy and society due to the ongoing climate crisis. For instance, the Renewable Energy Directive (Directive (EU) 2023/2413) sets the European Union renewable energy target to at least 42.5 % by 2030. With offshore renewables playing a key role in reaching this objective (111 GW by 2030), the demand on the seabed is increasing. A common challenge in exploiting such offshore resources is characterising and monitoring Europe’s variable and dynamic seabed which poses significant risks to the siting and installation of engineering structures. The fiscal implications of poor background knowledge of geological and geotechnical risk before construction onset are well demonstrated by previous projects in Europe. To promote the growth of this sector in a sustainable and economically efficient manner, alongside other existing and prospective industries, the development of integrated geo-spatial tools that facilitate the interrogation of key oceanographic and geological datasets to generate standardised indicators are paramount.

To date, the characterisation and description of sediment mobilisation and seabed disturbance has been carried out using a labour and expertise intensive process. This Project will develop a ‘Sediment mobility and seabed disturbance geo-spatial toolbox (Sed-mob-bed Tool)’, a time-saving, reliable and repeatable means of qualifying and quantifying sediment mobility for a range of sediment types. This novel Sed-mob-bed Tool will facilitate the interrogation of spatial oceanographic and sedimentological datasets to produce a set of standardised sediment mobility and seabed disturbance indices (e.g., Mobilisation Frequency Index (MFI), Seabed Disturbance Index (SDI) and Sediment Mobility Index (SMI)) applicable to international end-users. Several research questions will be addressed, including:

  • What are the key physical processes, sedimentological characteristics and parameters critical to sediment mobility?
  • What are the most effective geospatial tools to garner this information?
  • Can this be applied in a way that is geostatisically robust?
  • How well do these approaches perform (i) in differing seabed morphological settings, and (ii) at scale?

The developed tool will be tested under several different environmental and seabed conditions. This includes an application to Irish Waters as a case study, leveraging the wealth of existing national and European level datasets (e.g., INFOMAR, EPA, EMODnet, GSI, Marine Institute). The results of which will be of particular interest to a cross-disciplinary group of practitioners including marine archaeologists, oceanographers, marine geoscientists, and engineers. The methodology and results from this work will ultimately provide a scientific knowledge base for the sustainable growth of the marine economy.

How to cite: Creane, S., Totska, A., and Coughlan, M.: A new sediment mobility and seabed disturbance geo-spatial toolbox (Sed-mob-bed Tool), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18440, https://doi.org/10.5194/egusphere-egu25-18440, 2025.

Let us focus on a specific question that may has an ability to build an efficient method toward extracting significantly major ingredients of pre-active events going ahead of significant seismic activities. What is the common point at the state spaces of significant earthquakes of Türkiye in 1999 and 2023? The answer comes from some live but non-instrumented observations, those are devised privately. Those observations are related to both waveguide and cavity effects of natural and/or manmade significant structures replaced in both underground and/or atmosphere. The effects are studied on the electromagnetic wave propagation at significant pre-seismic activities of both circularly cylindrical wave guide and cavity structures meshed in underground and/or atmosphere by considering the extended wave equations in irregularly deviating environs1. Those structures have excessive dimensions as in subway tunnels2 and/or layered guiding pathways in atmosphere3.

The answer comes from two big tunnels excavated before abovesaid two earthquakes of Türkiye. First is Mount Bolu Tunnel, that is almost finished in 2007 and begun in 1993 and second is New Mount Zigana Tunnel, that is finished in 2023 and begun in 2016. Why? First of all, both tunnels are into mounts area of Northern Anatolia. The reason is related to the changing character of seismic activities after 5.9 R (included) magnitude that converts the seismic activities to electromagnetic activities majorantly4.

There is one more tunnel process that still continues for constructions: Between Bahce (37° 12′ 0″ N, 36° 35′ 0″ E) and Nurdagi (37° 10′ 44″ N, 36° 44′ 23″ E) districts of Gaziantep Province, Türkiye. This tunnel construction may have a potential on future seismic activities as two tunnel constructions said in previous paragraph.

The cavities and tunnels behave as layered guiding pathways for propagating waves either homogeneous and/or inhomogeneous fillings; therefore, the activities of waveforms may propagate along long distances under the Earth; i.e., between NAF and SAF by suitable transmissions, propagations, and guiding of waves. The majorant contributions come through Casimir and Casimir-like activities from the boundary interfaces between different materials with specific conditions under stochastic processes. The propagating waves create similar effects among transmitters and receivers through atmosphere layers. Author calls transmission effect by the cavity tunneling and layered guiding pathways these effects.

Those circumstances are studied in above paragraphs by considering the state space formulation of equivalent electrical circuits models through the possible mechanical circuits into the Earth.

The equivalent circuit model governs the significant Seismic Activities, sSAs, by the interactions among source and sink structures available in the distributed networks of equivalent circuits. New constructions have the ability to trigger and produce sSAs close to both specific domains of sSAs and their neighbor domains even if they never generated sSAs in past, of tunnel projects in paragraph 3 and similar ones. Temporal intervals may not coincide with the time spans of excavations of sSAs processes and their triggering effects may either decrease, mostly and/or increase, asymptotically as depending to coupling activities in environ.

 

1https://doi.org/10.1109/APS.1996.549734

2https://doi.org/10.5194/egusphere-egu2020-22589.

3 https://doi.org/10.1109/RAST.2003.1303999.

4 https://doi.org/10.5194/egusphere-egu2020-21121.

How to cite: Sengor, T.: The Cavity Tunneling and Layered Guiding Pathways in Significant Seismic Activities: Pre-fingerprints in Significant Earthquakes of Türkiye in 1999 and 2023, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-988, https://doi.org/10.5194/egusphere-egu25-988, 2025.

There has long been research on the phenomenon of abnormal microwave radiation emitted from the Earth's surface before a major earthquake. However, the enhanced microwave radiation received by satellite sensors is affected by a combination of factors such as surface vegetation, soil moisture, land surface temperature, and atmospheric environment. So far, it has been difficult to remove non-seismic interference through quantitative physical modeling, leaving only the earthquake-related additional components for earthquake precursor analysis and short-term earthquake prediction. To tackle with this, we developed a knowledge-guided deep learning model that leverages a large amount of remote sensing observation data for training, incorporating prior knowledge of earthquake anomaly analysis. In the modelling process, a large amount of multi-source data, such as surface microwave brightness temperature (MBT), land surface temperature (LST), surface vegetation index, soil moisture index, atmospheric water vapor content, cloud cover, land cover type, digital elevation model (DEM), and geological type, were collected, and a regression model between multiple factors and surface MBT were firstly established through deep learning methods. In the same way, another regression model was developed between non-temperature parameters and LST by using historical records. During the seismic window of one month before and after the target earthquake, the LST was obtained by using non-temperature data through the second regression model, and then was substituted it into the first regression model to get the MBT value that does not include the additional effects of earthquakes. Eventually, we can obtain the additional MBT value due to seismic activity by calculating the difference with the actual observation, which represents the earthquake-related MBT anomaly. Since the deep learning-based modeling is based on long time series data and the output results of the model already include the contribution of multiple factors on the surface to the MBT, the differential results are mainly affected by the additional impacts of the earthquake, so they can be considered 'pollution-free'. In other words, there is no need to use additional auxiliary data to discriminate and separate the non-seismic disturbances. For a specific target area, such as the Tibetan Plateau, after establishing a model based on historical data using the aforementioned method, we can obtain real-time earthquake MBT variations as the input data is continuously updated. This can be used to analyze and identify potential earthquake precursors, and consequently, for short-term earthquake prediction.

How to cite: Qi, Y., Mao, W., Wu, L., and Huang, B.: A Knowledge-Guided Deep Learning Model for Extracting Pollution-free Seismic Microwave Brightness Temperature Anomalies, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1408, https://doi.org/10.5194/egusphere-egu25-1408, 2025.

EGU25-2283 | Orals | NH4.4

On the Ionosphere-Atmosphere-Lithosphere coupling during theNovember 9, 2022 Italian Earthquake 

Mirko Piersanti, Giulia D'Angelo, Dario Recchiuti, Fabio Lepreti, Paola Cusano, Enza De Lauro, Vincenzo Carbone, Pietro Ubertini, and Mariarosaria Falanga

In the last decades, the scientific community has been focused on searching earthquake signatures in the Earth's atmosphere, ionosphere, and magnetosphere. This work investigates an offshore Mw 5.5 earthquake that struck off the Marche region's coast (Italy) on November 9, 2022, with a focus on the potential coupling between the Earth's lithosphere, atmosphere, and magnetosphere triggered by the seismic event. Analysis of atmospheric temperature data from ERA5 reveals a significant increase in potential energy (Ep) at the earthquake's epicenter, consistent with the generation of Atmospheric Gravity Waves (AGWs). This finding is further corroborated by the MILC analytical model, which accurately simulates the observed Ep trends (within 5%), supporting the theory of Lithosphere-Atmosphere-Ionosphere-Magnetosphere Coupling. The study also examines the vertical Total Electron Content (vTEC) and finds notable fluctuations at the epicenter, exhibiting periodicities (7-12 minutes) characteristic of AGWs and traveling ionospheric disturbances. The correlation between ERA5 observations and MILC model predictions, particularly in temperature deviations and Ep distributions, strengthens the hypothesis that earthquake-generated AGWs impacted atmospheric conditions at high altitudes, leading to observable ionospheric perturbations. This research contributes to a deeper understanding of Lithosphere-Atmosphere-Ionosphere-Magnetosphere Coupling mechanisms and the potential for developing reliable earthquake prediction tools.

How to cite: Piersanti, M., D'Angelo, G., Recchiuti, D., Lepreti, F., Cusano, P., De Lauro, E., Carbone, V., Ubertini, P., and Falanga, M.: On the Ionosphere-Atmosphere-Lithosphere coupling during theNovember 9, 2022 Italian Earthquake, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2283, https://doi.org/10.5194/egusphere-egu25-2283, 2025.

We discuss the potential impact of the Geospace environment on the significant earthquake preparation processes. In this work, we investigate the response of major seismic activity to geomagnetic storms with a joint analysis of solar wind, geomagnetic field, and earthquake catalog. As a test case, we processed the seven strongest earthquakes in Italy for the period  1980 - 2016:  Amatrice M6.2 of Aug 24, 2016; Visso M6.1 of 26 Oct 2016; Norcia M6.6 of 30 Oct 2016; Emilia-Romagnia M6 of May 20, 2012;  L’Aquila M6.3 of Apr 6, 2009;  Foligno M6 of Sep 26,1997  and  Irpina of M6.9 of 23 Nov 1980. All of the seismic events were preceded by geomagnetic storms, which satisfied a given criterion: at the time of geomagnetic storm onset, the high-latitude part of the longitudinal region, where in the future an earthquake occur, was located under the polar cusp, where the solar wind plasma would directly access the Earth’s environment [Ouzounov and Khachikyan, 2024]. The number of preceded storms varied for different earthquakes from two to five. This results in different time delays between the day of the magnetic storm onset and the day of earthquake occurrence; it ranges between 9-80 days. Because of the existing delay between a shocked solar wind arrival and earthquake occurrence up to some months, this may suggest that solar wind energy does not trigger earthquakes immediately (as it is believed at present); instead, it may accelerate the processes of lithosphere dynamics, such as fluid and gas upwelling, which are active participants in tectonic earthquakes. For comparison, we present the results of the same analysis applied to other territories of the Mediterranean region: the Anatolian Plate (Turkey) and Crete Island (Greece), which look strikingly similar.

 

How to cite: Ouzounov, D. and Khachikyan, G.: The impact of the geospace environment on earthquake preparation processes. Case studies for M>6 in Italy for 1980-2016, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3686, https://doi.org/10.5194/egusphere-egu25-3686, 2025.

EGU25-5269 | Orals | NH4.4

Similarities and differences of the preparation of three (M≈6) earthquake doublets around the Arabian Plate 

Essam Ghamry, Dedalo Marchetti, and Mohamed Metwaly

In this study, we compared the results of multiparametric and multilayers investigations of three doublet earthquakes that occurred around the Arabian plate (M6.2 + M6.0 on 18 August 2014 close to Dehloran, Iran; M6.0 + M6.0 occurred on 15 July 2018 offshore Kilmia, Yemen and M6.0 + M6.0 occurred on 1 July 2022 close to Bandar-e Lengeh). We applied identical methods to the same dataset for all three cases. In particular, we investigated lithospheric, atmospheric, and ionospheric data six months before the three events. The lithosphere was investigated by calculating the cumulative Benioff strain with the USGS earthquake catalogue. Several atmospheric parameters (aerosol, SO2, CO, surface air temperature, surface latent heat flux humidity, and dimethyl sulphide) have been monitored using the homogeneous data from the MERRA-2 climatological archive. We used the three-satellite Swarm constellation for magnetic data, analysing the residuals after removing a geomagnetic model. All the cases present some patterns of anomalies, and when comparing them, we noticed some similarities but also differences. We pointed out that the released energy by the three events is very similar and occurred around the same plate. Still, they involved two different tectonic contexts (compressional on the Iranian side and extensional and transcurrent on the African Plate border). For the above reasons, their comparison is very interesting. Some similarities seem to be explainable in the tectonic context, and some are caused by the ocean's influence at the epicentre location. However, we also identified some differences that still require further investigation and comparison with other case studies.

Finally, this work can be considered a preliminary test of an extensive investigation and systematical search of LAIC patterns before the earthquake occurrences and the study of the possible influence of focal mechanism, location, geological factors, and other constraints.

 

References :

Ghamry Essam; Marchetti Dedalo; Metwaly Mohamed. Geophysical Coupling Before Three Earthquake Doublets Around the Arabian Plate. Atmosphere 2024, 15, 1318. https://doi.org/10.3390/atmos15111318

 

How to cite: Ghamry, E., Marchetti, D., and Metwaly, M.: Similarities and differences of the preparation of three (M≈6) earthquake doublets around the Arabian Plate, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5269, https://doi.org/10.5194/egusphere-egu25-5269, 2025.

EGU25-5321 | Posters on site | NH4.4

Novel experimental design for the study of seismic processes based on the stick-slip mechanism. 

Alejandro Ramírez-Rojas, Luciano Telesca, and Elsa Leticia Flores-Márquez

Seismicity is the result of the interaction between tectonic plates in relative motion where the underlying mechanism of earthquake generation in seismic subduction areas is stick-slip. In reality, seismicity is a complex phenomenon as it involves processes that take place from within the Earth. A thorough understanding of seismicity requires theoretical and experimental approaches. The dynamics in subduction zones occur when two tectonic plates, one on top of the other, are in relative motion where the plate below is in motion due to convective processes within the Earth. Due to the roughness of both surfaces, the underlying mechanism that gives rise to seismicity is stick-slip. In this work, an experimental stick-slip model is proposed, which simulates the relative motion of two rough surfaces by the interaction of two blocks covered by sandpaper with a certain degree of roughness. In this experimental model, the interaction between rough surfaces (sandpaper), with a relative motion in opposite directions to each other, produces stick-slip events (synthetic seismicity), which mimic real seismicity. Here we present the first analyses of synthetic seismicity by calculating the Gutenberg-Richter law, temporal correlations and characterization in terms of organization and order from the Fisher-Shannon method for each synthetic catalogue.

How to cite: Ramírez-Rojas, A., Telesca, L., and Flores-Márquez, E. L.: Novel experimental design for the study of seismic processes based on the stick-slip mechanism., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5321, https://doi.org/10.5194/egusphere-egu25-5321, 2025.

EGU25-5493 | Orals | NH4.4

Toward Real-Time Forecasting of Earthquake Occurrence and Ground-Shaking Intensity Using ETAS and GMM: Insights from Recent Large Earthquakes in Taiwan 

Ming-Che Hsieh, Chung-Han Chan, Kuo-Fong Ma, Yin-Tung Yen, Chun-Te Chen, Da-Yi Chen, and Yi-Wun Liao

Earthquake forecasting, combined with precise ground-shaking estimations, plays a pivotal role in safeguarding public safety, fortifying infrastructure, and bolstering the preparedness of emergency services. This study introduces a comprehensive workflow that integrates the epidemic-type aftershock sequence (ETAS) model with a preselected ground-motion model (GMM), facilitating accurate short-term forecasting of ground-shaking intensity (GSI), which is crucial for adequate earthquake warning for earthquake-prone regions like Taiwan. First, an analysis was conducted on a Taiwanese earthquake catalog from 1994 to 2022 to optimize the ETAS parameters. The dataset used in this analysis allowed for the further calculation of total, background, and clustering seismicity rates, which are crucial for understanding spatiotemporal earthquake occurrence. Subsequently, short-term earthquake activity simulations were performed using these up-to-date seismicity rates to generate synthetic catalogs. The ground-shaking impact on the target sites from each synthetic catalog was assessed by determining the maximum intensity using a selected GMM. This simulation process was repeated to enhance the reliability of the forecasts. Through this process, a probability distribution was created, serving as a robust forecasting for GSI at sites. The performance of the forecasting model was validated through an example of the Taitung, Taiwan earthquake sequence in September 2022, showing its effectiveness in forecasting earthquake activity and site-specific GSI. The other example is the Hualien, Taiwan earthquake sequence from April 2024, which serves as an excellent demonstration of a workflow designed to provide real-time aftershock forecasting following an M7.2 event. The proposed forecasting model can quickly deliver short-term seismic hazard curves and warning messages, facilitating timely decision-making.

How to cite: Hsieh, M.-C., Chan, C.-H., Ma, K.-F., Yen, Y.-T., Chen, C.-T., Chen, D.-Y., and Liao, Y.-W.: Toward Real-Time Forecasting of Earthquake Occurrence and Ground-Shaking Intensity Using ETAS and GMM: Insights from Recent Large Earthquakes in Taiwan, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5493, https://doi.org/10.5194/egusphere-egu25-5493, 2025.

EGU25-8052 | Orals | NH4.4

Multiparameter observations of Lithosphere–Atmosphere–Ionosphere pre-seismic anomalies: Insights from the 2022 M6.8 Chihshang earthquake in southeastern Taiwan 

Ching-Chou Fu, Hao Kuo-Chen, Chung-Hsiang Mu, Hau-Kun Jhuang, Lou-Chuang Lee, Vivek Walia, and Tsung-Che Tsai

This study conducted a systematic analysis of the 2022 Chihshang earthquake sequence in eastern Taiwan, integrating multidimensional observational parameters related to the lithosphere, atmosphere, and ionosphere. High-resolution data from the MAGIC (Multidimensional Active fault of Geo-Inclusive observatory - Chihshang) at the Chihshang fault area provided a comprehensive and diverse dataset. The analysis revealed significant pre-earthquake anomalies across various parameters. These include a marked increase in soil radon concentration one month prior to the earthquake, concurrent anomalies in hydrogeochemical parameters (e.g., elevated groundwater temperature, reduced pH, and decreased chloride ion concentration), and active foreshock activity detected by a dense microseismic network starting mid-August, suggesting the development of microfractures within the lithosphere. Additionally, persistent OLR (Outgoing Longwave Radiation) anomalies, indicating hotspots near the epicenter, were observed from September 5 to 7. Pre-earthquake signals in TEC (Total Electron Content) were identified between August 20 and September 13 in two independent datasets, GIM-TEC and CWA-TEC.

Post-earthquake observations revealed a significant increase in CO2 flux in the region, likely attributable to the release of deep-seated gas sources or enhanced permeability of the fault system. These combined observations suggest that all anomalies can be classified as short-term precursors, which can be interpreted within the theoretical framework of lithosphere-atmosphere-ionosphere coupling (LAIC). The findings also contribute to a deeper understanding of the earthquake preparation process. This study underscores the critical importance of real-time integration of multi-parameter observations, offering new insights and improvements for seismic hazard assessment and advancing the predictive capability of earthquake precursors.

How to cite: Fu, C.-C., Kuo-Chen, H., Mu, C.-H., Jhuang, H.-K., Lee, L.-C., Walia, V., and Tsai, T.-C.: Multiparameter observations of Lithosphere–Atmosphere–Ionosphere pre-seismic anomalies: Insights from the 2022 M6.8 Chihshang earthquake in southeastern Taiwan, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8052, https://doi.org/10.5194/egusphere-egu25-8052, 2025.

EGU25-8652 | ECS | Posters on site | NH4.4

Recent achievements on the application of Robust Satellite Techniques to the short-term seismic hazard forecast 

Roberto Colonna, Carolina Filizzola, Nicola Genzano, Mariano Lisi, Iacopo Mancusi, Carla Pietrapertosa, and Valerio Tramutoli

Robust Satellite Techniques applied to long-term satellite TIR (Thermal InfraRed) radiances have
been, since more than 25 years, employed to identify those anomalies (in the spatial/temporal
domain) possibly associated to the occurrence of major earthquakes.
The results until now achieved by processing multi-annual (more than 10 years) time series of TIR
satellite images collected in different continents and seismic regimes, showed that more than 67%
of all identified (space-time persistent) anomalies occur in the pre-fixed space-time window around
the occurrence time and location of earthquakes (M≥4), with a false positive rate smaller than 33%.
Moreover, Molchan error diagram analysis gave a clear indication of non-casualty of such a
correlation, in comparison with the random guess function.
After the most comprehensive test performed over Greece, Italy, Turkey and Japan, here, we will
critically discuss the preliminary results achieved over California by applying RST analyses to
long-term series of GOES-17 radiances.

How to cite: Colonna, R., Filizzola, C., Genzano, N., Lisi, M., Mancusi, I., Pietrapertosa, C., and Tramutoli, V.: Recent achievements on the application of Robust Satellite Techniques to the short-term seismic hazard forecast, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8652, https://doi.org/10.5194/egusphere-egu25-8652, 2025.

EGU25-8809 | Orals | NH4.4

Noise reductions of VLF signals and excitation/attenuation of waves with small wave periods before earthquakes 

Giovanni Nico, Aleksandra Nina, Pierfrancesco Biagi, Hans Ulrich Eichelberger, Mohammed Y. Boudjada, and Luka Č. Popović

Various types of changes in the characteristics of very low frequency (VLF) signals before earthquakes have been presented during the past few decades. Most of these changes have been observed on data with time sampling of the order of a few tenths of a second or of the order of minutes. Improvements in this sampling in recent years have indicated three new types of changes whose onsets have been observed a few minutes or tens of minutes before the earthquake. These changes manifest themselves as reductions in the VLF signal amplitude and phase noises, and excitation and attenuation of waves with small wave periods in both of these signal characteristics [1-5].

In this work, we present these changes and list the parameters in the time and frequency domains that are significant for statistical analyses. A central issue is the relationship of the changes with the characteristics of earthquakes, the observed signals, and their spread in the surrounding area. The presented analyses were conducted on data recorded by a VLF receiver in Belgrade, Serbia.

 

References:

[1] A. Nina, S. Pulinets, P.F. Biagi, G. Nico, S.T. Mitrović, M. Radovanović, L.Č. Popović, “Variation in natural short-period ionospheric noise, and acoustic and gravity waves revealed by the amplitude analysis of a VLF radio signal on the occasion of the Kraljevo earthquake (Mw = 5.4)”, Science of The Total Environment, 710, 136406, 2020.

[2] A. Nina, P. F. Biagi, S. T. Mitrović, S. Pulinets, G. Nico, M. Radovanović,  L. Č. Popović, “Reduction of the VLF signal phase noise before earthquakes”, Atmosphere 12 (4), 444, 2021.

[3] A. Nina, P. F. Biagi, S. A. Pulinets, G. Nico, S. T. Mitrović, V. M. Čadež, M. Radovanović, M. Urošev,  L. Č. Popović, “Variation in the VLF signal noise amplitude during the period of intense seismic activity in Central Italy from 25 October to 3 November 2016”, Frontiers in Environmental Science, 10, 10:1005575, 2022.

[4] A. Nina, “Analysis of VLF Signal Noise Changes in the Time Domain and Excitations/Attenuations of Short-Period Waves in the Frequency Domain as Potential Earthquake Precursors”, Remote Sensing, 16(2), 397, (2024)

[5] A. Nina “VLF Signal Noise Reduction during Intense Seismic Activity: First Study of Wave Excitations and Attenuations in the VLF Signal Amplitude”, Remote Sensing, 16(8), 1330, 2024.

 

How to cite: Nico, G., Nina, A., Biagi, P., Eichelberger, H. U., Boudjada, M. Y., and Popović, L. Č.: Noise reductions of VLF signals and excitation/attenuation of waves with small wave periods before earthquakes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8809, https://doi.org/10.5194/egusphere-egu25-8809, 2025.

A critical review of geoelectrical monitoring activities carried out in seismically active areas is presented and discussed. The electrical resistivity of rocks is one of the geophysical parameters of greatest interest in the study of possible seismic precursors, and it is strongly influenced by the presence of highly fractured zones with high permeability and fluid levels. The analysis in this study was based on results obtained over the last 50 years in seismic zones in China, Japan, the USA and Russia. These previous works made it possible to classify the different monitoring strategies, to analyze the theoretical models for interpreting possible correlations between anomalies in resistivity signals and local seismicity, and to identify the main scientific and technological gaps. In addition, much attention is given to some recent work on the study of correlations between focal mechanisms and the shapes of anomalous patterns in resistivity time series, and to the new possibilities offered by the AI-based methods for geophysical data processing. Finally, new strategies and activities for investigating the spatial and temporal dynamics of the electrical resistivity changes in seismically active areas were identified.

How to cite: Lapenna, V.: Detecting DC Electrical Resistivity Changes in Seismic Active Areas: State-of-the-Art and Future Directions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9250, https://doi.org/10.5194/egusphere-egu25-9250, 2025.

EGU25-9938 | ECS | Posters on site | NH4.4

High resolution tsunami inundation maps: towards multi-hazard risk analysis. 

Hany M. Hassan and Antonella Peresan

Multi-hazard disaster risk analyses in coastal areas requires the integration of data and models concerning hazard, exposure and vulnerability data and models, all developed with high spatial resolution. Indeed, accurate high-resolution models and data are essential for properly assessing the impact of specific hazards that threaten coastal areas, such as tsunamis, floods, landslides, and coastal erosion. Nevertheless, this level of detail remains unachieved for many coastal hazards in various locations. Consequently, critical fine-scale differences in localized risk assessment are overlooked, leading to potential underestimations or overestimations of the actual risk to coastal communities. It is vital to address this gap in order to enhance the accuracy and reliability of risk assessments.

A key step in tsunami hazard and risk assessment involves the development of inundation maps, specifically maps describing inundated areas and related depths. To date, such maps are not yet available at proper resolution for the coastal areas of the Friuli-Venezia-Giulia Region (FVG). Accordingly, this study aims to enhance the characterization of tsunami hazard in the Northern Adriatic by developing detailed inundation maps and possibly addressing the identified research gaps. Leveraging on accurate and high resolution bathymetry and topographic data is crucial for reliable tsunami modelling for the FVG coastal areas. To this purpose, bathymetry and topographic data are refined and are used, along with existing databases of tsunamigenic earthquake sources, for modelling tsunami waves propagation and inundation by means of the NAMI DANCE code (e.g. Yalciner et al. 2014, Mediterranean Sea Oceanography and references therein).

Existing datasets from open access and local data sources are collected and then refined, particularly addressing inaccuracies in lagoon bathymetry. This involves incorporating high-resolution data and considering small-scale coastal features that can significantly impact tsunami inundation. Multiple bathymetry and topography datasets are used to develop high resolution refined data at 25 meters, and 10 meters resolution. The database of co-seismic seafloor displacement for all individual scenarios, developed based upon the DISS-3.3.0 database, is adopted to carry out a reappraisal of tsunami wave amplitude maps (Peresan & Hassan, MEGR 2024 and references therein) and to estimate realistic tsunami inundation maps. Additionally, tsunami sources caused by local earthquakes relevant to the FVG region are investigated, providing local scale maps of wave amplitudes and inundation estimates; this involves using appropriate fault rupture realisations for local tsunami scenarios (ITCS100&101), as specified in the DISS-3.3.0 database.

The outcomes from this study provide the basis for multi-scenario tsunami hazard assessment, contributing to the development of high-resolution and comprehensive tsunami hazard maps for the Northern Adriatic coasts. Moreover, along with high-resolution exposure maps, they contribute improving precision and accuracy of related risk assessment, and hence are an important step in preparedness, response, and prevention efforts in the framework of disaster risk management.

This research is a contribution to the RETURN Extended Partnership (European Union Next-Generation EU—National Recovery and Resilience Plan—NRRP, Mission 4, Component 2, Investment 1.3—D.D. 1243 2/8/2022, PE0000005).

How to cite: Hassan, H. M. and Peresan, A.: High resolution tsunami inundation maps: towards multi-hazard risk analysis., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9938, https://doi.org/10.5194/egusphere-egu25-9938, 2025.

EGU25-10351 | Posters on site | NH4.4

Investigation of VLF/LF electromagnetic wave propagation as recorded by the receivers of the INFREP network 

Iren-Adelina Moldovan, Victorin Emilian Toader, Hans Ulrich Eichelberger, Pier Francesco Biagi, Mohammed Boudjada, Mihai Anghel, Liviu Marius Manea, Andrei Mihai, and Bogdan Antonescu

In recent decades, significant efforts have been devoted to understanding and interpreting the link between ionospheric perturbations and natural or anthropogenic phenomena, such as seismic activity, electrical or geomagnetic storms, and unidentified radio emissions. This is achieved through various methods among which is also the study of electromagnetic (EM) wave propagation in the very low frequency (VLF, 3–30 kHz) and low frequency (LF, 30–300 kHz) bands. These bands enable long-distance communication, navigation, and military applications, including submarine contact, AM broadcasting, lightning detection, and weather systems. Due to their long wavelengths, VLF and LF waves exhibit unique propagation characteristics. VLF waves propagate globally by using Earth-ionosphere waveguides, reflecting off the D and E layers as skywaves, and are influenced by solar and atmospheric conditions. LF waves primarily rely on ground waves for extensive coverage, although they can also utilize ionospheric reflection (skywaves) for longer-distance communication.

This paper introduces fundamental concepts related to VLF/LF electromagnetic wave emission, propagation, reception, and the perturbing factors that affect them. Additionally, it presents key findings from the European INFREP Receivers Network, which studies seismo-ionospheric anomalies linked to earthquake activity. Established in 2009, the INFREP network monitors VLF/LF signals from transmitters across Europe and neighboring regions. The network currently comprises 10 receivers, built by Elettronika (Italy), and operates at a sampling rate of one sample per minute. The Romanian segment of INFREP includes two receivers, operational since 2009 and 2017, with only brief interruptions, notably during the pandemic when travel restrictions hindered access to the observatories.

The paper discusses the current state of the INFREP network and outlines methods for providing near real-time data access. It highlights advancements in real-time electromagnetic data transmission, archiving, and the use of 2D and 3D online signal visualization and processing techniques. Data access is available through the INFREP headquarters in Graz, Austria (https://infrep.iwf.oeaw.ac.at/data-access/) and the National Institute for Earth Physics in Romania (https://mg.infp.ro/d/ch-aqZXIz/vlf-lf-radio-data?orgId=1&from=now-6M&to=now). The paper also shares findings from the detection of potential ionospheric anomalies in EM signals preceding large earthquakes that occurred between 2012 and 2024. All anomalies are analyzed in correlation with space weather events and extreme meteorological phenomena.

This paper was carried out within Nucleu Program SOL4RISC, supported by MCI, project no PN23360201, and PNRR- DTEClimate Project nr. 760008/31.12.2023, Component Project Reactive, supported by Romania - National Recovery and Resilience Plan

 

How to cite: Moldovan, I.-A., Toader, V. E., Eichelberger, H. U., Biagi, P. F., Boudjada, M., Anghel, M., Manea, L. M., Mihai, A., and Antonescu, B.: Investigation of VLF/LF electromagnetic wave propagation as recorded by the receivers of the INFREP network, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10351, https://doi.org/10.5194/egusphere-egu25-10351, 2025.

EGU25-10353 | ECS | Orals | NH4.4

High-resolution exposure models for coastal cities in Northern Adriatic for multi-risk analysis 

Hazem Badreldin, Chiara Scaini, Hany M Hassan, and Antonella Peresan

Multi-hazard disaster risk reduction and mitigation require high-resolution exposure models that grasp the characteristics of assets at the local scale. High-resolution exposure models may allow improving precision/accuracy of risk and damage assessments, especially for hazards which are characterised by high spatial variability or may be influenced by the presence of the assets, such as tsunami or flooding. We propose a methodology for developing a high-resolution population and residential buildings exposure models, to be used for multi-hazard risk reduction purposes at the local scale.  This method has been tested and validated for a selected coastal area in the upper Adriatic, exposed to multiple hazards including earthquakes, tsunamis, meteorological events and coastal erosion. For the development of the population exposure model, a high-resolution population density data, collected at global scale, is combined with the national population census data, leveraging  both on the accuracy of the national census and on the resolution of the global data. Also, the building census data is complemented with exposure indicators extracted from digital building footprints from the Carta Tecnica Regionale Numerica (CTRN),  which is missing in census data, such as average built area, total built area, replacement cost, height and plan regularity. The final exposure layers are assembled at two resolutions: 100 meters and 30 meters, with information also provided at the census unit level. We discuss the development and use of these layers for multi-risk assessment and their potential combination with artificial intelligence. 

This research is a contribution to the projects: RETURN Extended Partnership (European Union Next-Generation EU—National Recovery and Resilience Plan—NRRP, Mission 4, Component 2, Investment 1.3—D.D. 1243 2/8/2022, PE0000005); PRIN-PNRR project SMILE: Statistical Machine Learning for Exposure development, funded by the European Union- Next Generation EU, Mission 4 Component 1 (CUP F53D23010780001). 

How to cite: Badreldin, H., Scaini, C., M Hassan, H., and Peresan, A.: High-resolution exposure models for coastal cities in Northern Adriatic for multi-risk analysis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10353, https://doi.org/10.5194/egusphere-egu25-10353, 2025.

Japan is frequently hit by major earthquakes, such as the 2011 off the Pacific coast of Tohoku Earthquake and the 2024 Noto Peninsula Earthquake, which cause enormous human and economic losses. Short-term forecast of earthquakes is effective for mitigating such damage, but this has not been achieved to date. On the other hand, there have been reports of electromagnetic phenomena preceding major earthquakes in various frequency bands, including precursor phenomena in the VLF/LF band (3-300 kHz). In this study, we investigated earthquake-related VLF/LF signals, which has strong electromagnetic emissions due to lightning activity, and it is important to discriminate the VLF/LF signals from those due to lightning activity. In this study, two approaches were attempted: (1) development of a source localization method using VLF/LF broadband interferometry and (2) removal of signals caused by lightning discharges using machine learning.
The first approach is expected to spatially discriminate between VLF/LF signals related to earthquakes (which are located near the epicenter and do not move) and signals related to lightning activity (which move with fronts and thunderclouds). The second is to utilize machine learning technology, which has been rapidly developed in recent years, for detection and removal of lightning discharge signals. For example, Wu et al. at Gifu University have succeeded in classifying lightning discharge waveforms in the thunderstorm activity process with an accuracy of approximately 99% using a machine learning technique called Random Forest. In this study, machine learning is expected to efficiently discriminate and eliminate known lightning discharge signals from a large amount of observation data with high accuracy, and analyze the remaining unknown signals to efficiently investigate the relationship between lightning and earthquakes. In this paper, we will describe the specific methods and results of the above two approaches.

How to cite: Hattori, K., Ota, Y., Yoshino, C., and Imazumi, N.: Construction of a VLF/LF band interferometer using a capacitive circular flat-plane antenna and discrimination and identification of observed VLF/LF band signals by machine learning: Preliminary results, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10447, https://doi.org/10.5194/egusphere-egu25-10447, 2025.

EGU25-13142 | Orals | NH4.4

Sub-ionospheric VLF/LF waveguide electric field investigation from Mw≥5.0 earthquake events with multiple receivers in Europe 

Hans U. Eichelberger, Mohammed Y. Boudjada, Aleksandra Nina, Bruno P. Besser, Daniel Wolbang, Maria Solovieva, Pier F. Biagi, Patrick H. M. Galopeau, Christoph Schirninger, Iren-Adelina Moldovan, Giovanni Nico, Manfred Stachel, Özer Aydogar, Cosima Muck, Josef Wilfinger, and Irmgard Jernej

Electric field amplitude and phase measurements between narrowband VLF/LF transmitters and receivers in the sub-ionospheric waveguide are affected and altered by man-made and natural sources (Nina 2024; Boudjada et al., 2024a,b). In this study we investigate Mw≥5.0 earthquakes (EQs) which occurred in Europe during the year 2024 based on data from the INFREP receiver network (Biagi et al., 2019; Moldovan et al., 2015; Galopeau et al., 2023). In the selected Mediterranean area with geographical longitude [-10°E, 40°E] and latitude [30°N, 50°N] the United States Geological Survey EQ catalog (USGS, 2025) provides 20 events with Mw≥5.0. For these EQs we apply the night-time amplitude method and consider variations in the terminator times (Hayakawa et al., 2010). The main radio links that cross the EQ prone areas are from transmitters localized in the southern part of Europe, including TBB (26.70 kHz, Bafa, Turkey), ITS (45.90 kHz, Niscemi, Sicily, Italy), and ICV (20.27 kHz, Tavolara, Italy). 

We find statistically significant electric field anomalies for various VLF/LF paths, particularly for events with higher magnitudes. The continuous VLF/LF electric field amplitude and phase datasets can be important parameters for real-time observations and services to assess seismic hazards and disturbing physical phenomena within the waveguide.

References:

Biagi, P.F., et al., The INFREP network: Present situation and recent results, OJER, 8, 101-115, 2019. https://doi.org/10.4236/ojer.2019.82007

Boudjada, M.Y., et al., Unusual sunrise and sunset terminator variations in the behavior of sub-ionospheric VLF phase and amplitude signals prior to the Mw7.8 Turkey Syria earthquake of 6 February 2023, Remote Sens., 16, 4448, 2024. https://doi.org/10.3390/rs16234448

Boudjada, M.Y., et al., Analysis of pre-seismic ionospheric disturbances prior to 2020 Croatian earthquakes, Remote Sens., 16, 529, 2024. https://doi.org/10.3390/rs16030529

Galopeau, P.H.M., et al., A VLF/LF facility network for preseismic electromagnetic investigations, Geosci. Instrum. Method. Data Syst., 12, 231–237, 2023. https://doi.org/10.5194/gi-12-231-2023

Hayakawa, M., et al., A statistical study on the correlation between lower ionospheric perturbations as seen by subionospheric VLF/LF propagation and earthquakes, JGR Space Physics, 115(A9), 09305, 2010. https://doi.org/10.1029/2009JA015143

Moldovan, I.A., et al., The development of the Romanian VLF/LF monitoring system as part of the International Network for Frontier Research on Earthquake Precursors (INFREP), Romanian Journal of Physics, 60 (7-8), 1203-1217, 2015. Bibcode: 2015RoJPh..60.1203M https://rjp.nipne.ro/2015_60_7-8/RomJPhys.60.p1203.pdf

Nina, A., VLF signal noise reduction during intense seismic activity: First study of wave excitations and attenuations in the VLF signal amplitude, Remote Sens., 16, 1330, 2024. https://doi.org/10.3390/rs16081330

USGS, United States Geological Survey earthquake catalog, https://www.usgs.gov/programs/earthquake-hazards, as of Jan 2025.

How to cite: Eichelberger, H. U., Boudjada, M. Y., Nina, A., Besser, B. P., Wolbang, D., Solovieva, M., Biagi, P. F., Galopeau, P. H. M., Schirninger, C., Moldovan, I.-A., Nico, G., Stachel, M., Aydogar, Ö., Muck, C., Wilfinger, J., and Jernej, I.: Sub-ionospheric VLF/LF waveguide electric field investigation from Mw≥5.0 earthquake events with multiple receivers in Europe, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13142, https://doi.org/10.5194/egusphere-egu25-13142, 2025.

EGU25-13210 | Orals | NH4.4

Comparative multifractal study of seismicity in two seismic zones of Türkiye in the period from 2010 to 2024. 

Elsa Leticia Flores-Marquez, Alejandro Ramirez Rojas, and Jennifer Pérez-Oregon

Intense earthquakes have been natural phenomena that produce enormous disasters, mainly in large urban areas, due to the intense energy released in a very short period. Earthquakes are inevitable natural phenomena, and up to now, they cannot be predicted. On February 6, 2023, a M 7.8 earthquake occurred in southern Türkiye, near the northern border of Syria. This earthquake was followed by a M 7.5 earthquake to the north. The relative motions of three major tectonic plates (Arabian, Eurasian, and African) and one smaller tectonic block (Anatolian) are responsible for the seismicity in Türkiye. Recently, Onur investigated the aftershock distribution and its relation to energy release on the faults and Coulomb stress change areas, his study allowed the relocation of two-catastrophic earthquakes. In the present work we analyze the behavior of multifractality and its complexity parameters calculated from the catalog of seismic magnitudes during a period of 14 years monitored within two regions of Türkiye: the first one (west) between (35-42) Latitude, (25-34) Longitude and the second one (East) between (35-42) Latitude and (34-42) Longitude, being this area where the doublet occurred. Our results show differences in both multifractality and its complexity measures between the two regions. These findings may be indicators of expected seismicity in each region.

 

How to cite: Flores-Marquez, E. L., Ramirez Rojas, A., and Pérez-Oregon, J.: Comparative multifractal study of seismicity in two seismic zones of Türkiye in the period from 2010 to 2024., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13210, https://doi.org/10.5194/egusphere-egu25-13210, 2025.

EGU25-14706 | Orals | NH4.4

Design of the PRELUDE CubeSat for investigating ionospheric D-region earthquake precursor 

Masashi Kamogawa, Masashiko Yamazaki, and Nagisa Sone

Despite advances in satellite remote sensing, predicting large earthquakes, remains a significant challenge due to the unpredictable nature of these events. To address this challenge, our study, building upon the achievements of the French DEMETER satellite, focuses on atmospheric and space electrical variations as potential indicators of ionospheric D-region precursors to earthquakes. This approach is expected to contribute to the enhancement of short-term prediction capabilities. For this purpose, we would like to introduce our CubeSat PRELUDE (Precursory electric field observation CubeSat Demonstrator), a tiny satellite dedicated to the earthquake precursor detection and elucidated the physical mechanism. PRELUDE is scheduled for launch in JFY2025 as part of JAXA’s Innovative Satellite Technology Demonstration Program. This study presents the results of the system design, development, and mission planning of the PRELUDE, aimed at clarifying the physical mechanisms behind the statistically significant earthquake precursor ionospheric phenomena. PRELUDE is a 6U CubeSat specialized in VLF electromagnetic wave intensity observation, weighing 8 kg. To achieve miniaturization, it incorporates a drive recording function to downlink only the data surrounding the EQ epicenter to ground stations, reducing data storage and transmission requirements. Additionally, it hybridizes the Langmuir and electric field probes, typically found on satellites weighing over 100 kg like DEMETER, into a compact design suitable for CubeSats weighing just a few kilograms. The hybrid sensor unit extends booms bidirectionally by 1.5 m from the satellite using a folding extension mechanism, In this presentation, we show the satellite design requirements for elucidating the mechanism of earthquake precursor phenomena.

How to cite: Kamogawa, M., Yamazaki, M., and Sone, N.: Design of the PRELUDE CubeSat for investigating ionospheric D-region earthquake precursor, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14706, https://doi.org/10.5194/egusphere-egu25-14706, 2025.

EGU25-14734 | Posters on site | NH4.4

Rapid prediction method of earthquake damage to masonry structures based on machine learning 

Lingxin Zhang, Yan Liu, Li Liu, and Baijie Zhu

Masonry structures are one of the most vulnerable to severe and extensive damage in terms of previous earthquakes. It is significant to quickly evaluate the seismic damage levels of masonry structures, to reduce casualties and economic losses caused by earthquakes. However, traditional methods based on manual judgment or finite element simulations tend to be relatively slower . In this paper, a machine learning-based rapid prediction method was proposed for assessing the seismic damage of masonry structures. By analysis of building data from several cities and combining ground motion with structural characteristics, 11 impact factors were identified as input variables. The LM-BP neural network model was developed by a backpropagation (BP) neural network with strong nonlinear modeling capabilities, and by the Levenberg-Marquardt (LM) algorithm. The accuracy and stability of the model were verified by comparing the predicted values with actual earthquake examples. The results show that the selected seismic damage impact factors can accurately reflect the structural damage level. By comparing methods using parameters on either the structure or ground motion, the predictive accuracy of the proposed method is significantly enhanced. It provides a basis for post-earthquake structural safety assessments and disaster prevention and mitigation work.

How to cite: Zhang, L., Liu, Y., Liu, L., and Zhu, B.: Rapid prediction method of earthquake damage to masonry structures based on machine learning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14734, https://doi.org/10.5194/egusphere-egu25-14734, 2025.

EGU25-16143 | ECS | Orals | NH4.4

Machine Learning based EStimator for ground shaking maps workflow applied to New Zealand 

Rut Blanco Prieto, Marisol Monterrubio Velasco, Brendon Bradley, Claudio Schill, and Josep de la Puente

Earthquakes are among the most frequent yet unpredictable natural hazards, posing substantial risk to human safety and infrastructure globally, particularly, when large-magnitude earthquakes occur. This highlights the urgent need to develop innovative and alternative methodologies for rapidly assessing the intensity of ground shaking following an earthquake.

This study explores the application of the Machine Learning Estimator for Ground Shaking Maps (MLESmap) methodology in New Zealand, a region characterized by  high seismic activity.

MLESmap utilizes extensive datasets of high-fidelity, physics-based seismic scenarios to rapidly estimate ground-shaking intensity in near real-time following an earthquake. This methodology has demonstrated evaluation times similar to those of empirical ground motion models, while offering superior predictive accuracy in the two previously tested regions: the Los Angeles basin and the South Iceland Seismic Zone (SISZ).

To adapt MLESmap for New Zealand’s seismicity, seismic simulations tailored to the unique geological and tectonic context of the region are implemented. Specifically, we use the dataset generated by CyberShake NZ, a probabilistic seismic hazard analysis (PSHA) software developed by the University of Canterbury. Using this software, a total of 11,362 finite-fault rupture simulations were performed across the region and seismic hazard results were calculated on a grid of 27,481 synthetic seismic stations. A ‘forward’ simulation approach was adopted due to the large number of output locations relative to rupture locations, the optimisation of the grid for each rupture and the intention to include plasticity.

The expected results aim to demonstrate the applicability of MLESmap to New Zealand, providing ML-based tools for rapid response actions. This study also takes the first steps in applying cascading effects to MLESmap, in order to improve the overall risk assessment and to advance prevention efforts through innovative and multidisciplinary methodologies.

 

 

©2023 ChEESE-2P Funded by the European Union. This work has received funding from the European High Performance Computing Joint Undertaking (JU) and Spain, Italy, Iceland, Germany, Norway, France, Finland and Croatia under grant agreement No 101093038.

How to cite: Blanco Prieto, R., Monterrubio Velasco, M., Bradley, B., Schill, C., and de la Puente, J.: Machine Learning based EStimator for ground shaking maps workflow applied to New Zealand, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16143, https://doi.org/10.5194/egusphere-egu25-16143, 2025.

The region near the India-Eurasia plate boundary has a long history of large earthquakes. Over the past century, more than 50 earthquakes with magnitudes of 7 or greater have occurred within 500 km of the Indo-Eurasian collision zone. These include the 2015 M7.8 Nepal earthquake, the 1934 M8.0 Bihar-Nepal earthquake, the 1950 M8.6 Assam earthquake, and the 1905 M7.9 Kangra earthquake. The January 7, 2025, M7.1 earthquake in the southern Tibetan Plateau further underscores the seismic significance of this region. This study examines the temporal variation in seismicity within the Indo-Eurasian collision zone and its adjacent areas by utilizing historical records and instrumentally recorded earthquake data from 1900 to 2024. Based on seismic behaviour, clustering of events, and tectonic structures, the collision zone is divided into 26 distinct seismic zones. The temporal variation in seismicity for each zone is analyzed, and a susceptibility index, ESI6, is calculated. This index considers the return period of earthquakes with Mw ≥ 6 and the time elapsed since the last Mw ≥ 6 earthquake in each zone. The ESI6 represents the number of pending Mw ≥ 6 earthquakes in each seismic zone. Ten zones with high ESI6 values (>2.5) have been identified; these zones were seismically active in the past but have remained without major earthquakes for the last three decades. To mitigate potential losses and raise awareness, it is critical to implement GPS monitoring of plate movements, satellite-based deformation monitoring, and seismic health assessments of crucial infrastructure in these silent zones.

How to cite: Kumar, S.: Spatio Temporal Analysis of Earthquake Potential in the Indo-Eurasian Collision Zone: Identifying Future Seismic Hotspots Using the Earthquake Susceptibility Index, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16591, https://doi.org/10.5194/egusphere-egu25-16591, 2025.

EGU25-17662 | Orals | NH4.4

Automated Site Effects Mapping in Mayotte Using Airborne Electromagnetic Data and Machine Learning 

Cécile Gracianne, Hugo Breuillard, Célia Mato, Pierre-Alexandre Reninger, Agathe Roullé, Anne Raingeard, and Roxanne Rusch

Recent seismic hazard assessments in Mayotte have highlighted the island's significant exposure to site effects during earthquakes. These effects are closely linked to its complex geological setting, characterized by altered volcanic formations whose heterogeneous geometry leads to strong spatial variations in ground motion. In response to governmental requests, a site effects map is being developed to raise public awareness and support risk-informed urban planning.

A novel methodology for site effects mapping has recently been developed at BRGM, integrating airborne electromagnetic (AEM) data with borehole logs, geological maps, and seismic data (MASW and H/V measurements). This approach was tested on three test sites covering 12 km² of Mayotte surface, and it has demonstrated its potential in imaging the geological interfaces responsible for site effects. However, the current methodology relies on expert-driven data interpretation, making its large-scale application highly labour-intensive and costly. To overcome this limitation, partial automation of the data processing is required in order to handle larger datasets efficiently.

Machine learning techniques offer a promising solution to address this challenge. The test sites provided a unique training dataset, associating resistivity profiles derived from AEM data with the position of geological interfaces responsible for site effects within the soil column. These interface locations were determined through the integration and interpretation of all available geological and geophysical data, including MASW, H/V measurements, and borehole logs. Using this dataset, we trained various models, including Random Forest and Convolutional Neural Networks (CNN), to predict the localization of geological interfaces responsible for site effects based on AEM data.

Preliminary results indicate that the CNN model shows good performances on this task. Nevertheless, further improvements require the expansion of training datasets, underscoring the significant investment needed to generalize this approach to other regions. Future research will focus on refining predictive models and optimizing data acquisition to support large-scale implementation.

How to cite: Gracianne, C., Breuillard, H., Mato, C., Reninger, P.-A., Roullé, A., Raingeard, A., and Rusch, R.: Automated Site Effects Mapping in Mayotte Using Airborne Electromagnetic Data and Machine Learning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17662, https://doi.org/10.5194/egusphere-egu25-17662, 2025.

Finding a sustainable solution to disaster risk mitigation needs to consider different aspects of the disaster’s impact along with social, economic, and physical characteristics of the region. In this regard, a desirable solution for disaster risk mitigation for a region is the one tailored to the local characteristics. These local characteristics not only help measure the different aspects of a disaster impact but also portray existing pressing issues as priorities. While the former can be modeled using risk and resilience assessment models, the latter can be measured from experts’ points of view. Ultimately, the combination of the expert’s perception on important issues and the output of risk and resilience assessment models can be used to evaluate the optimality of each disaster risk mitigation solution.

In this research, a Multi-Criteria Decision Analysis (MCDA) framework is developed to provide an evaluation of each disaster risk mitigation. The developed framework is designed to be able to run on the action-outcome results from risk and resilience assessment models and the cardinal ranking of the decision criteria, representing decision-makers’ expert opinion on the priorities in mitigating and managing disaster risk. The developed MCDA framework is very practical as it can run on action-outcome results, and these results are accessible from a large variety of risk and resilience assessment models. Furthermore, the developed MCDA framework takes into account the uncertainty in the risk and resilience assessment models. In compatibility with running on minimal available information, the MCDA’s decision model is simplified to one layer with a single layer of the decision criteria.

Additionally, as the number of competing mitigation solutions might increase rapidly in practice, the MCDA framework is developed to handle a huge number of alternatives more efficiently and with relatively limited computational resources. The MCDA framework is developed based on the CAR method of eliciting the preferences among mitigation alternatives. The final results evaluate the competing disaster risk mitigation solution based on available data (as processed by risk and resilience assessment models) and the expert’s opinion on important issues and their preferences on the important aspects of disaster impact. As such, the final results provide an estimation of the expert’s belief on the desirability of each of the disaster risk mitigation solutions.

This MCDA framework is developed as part of the Horizon Europe project MEDiate (Multi-hazard and risk-informed system for Enhanced local and regional Disaster risk management). This project is dedicated to creating a decision-support system (DSS) for disaster risk management that not only takes into account the complexities of multiple interacting natural hazards but also tailors the final solution to the characteristics, priorities, and concerns of the local communities and decision-makers. The MEDiate framework is implemented on four different testbeds (Oslo (Norway), Nice (France), Essex (UK), and Múlaþing (Iceland)), each of which has a different multi-hazard pair and different socio-economic characteristics. The deployment of the developed MCDA framework on different natural hazards and socio-economic characteristics shows its flexible practicality.

How to cite: Yeganegi, M. R., Komendantova, N., and Danielson, M.: Measuring the experts’ perception about the suitability of natural disaster risk mitigation solutions using minimal risk assessment information, a Multi-Criteria Decision Analysis approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17936, https://doi.org/10.5194/egusphere-egu25-17936, 2025.

EGU25-18225 | Posters on site | NH4.4

A web platform for crowdsourced collection, processing, and visualization of exposure data on buildings 

Maria Teresa Artese, Elisa Varini, Isabella Gagliardi, Gianluigi Ciocca, Flavio Piccoli, Claudio Rota, Matteo Del Soldato, Silvia Bianchini, Chiara Scaini, Antonella Peresan, and Piero Brondi

The ultimate objective of our research is to explore the potential of Machine Learning in the dynamic creation of up-to-date exposure layers for buildings. This effort involves integrating remote sensing images, ancillary data such as national census information, and crowdsourced data collected by trained citizens. The crowdsourcing activity builds on a previous successful initiative developed within the CEDAS (building CEnsus for seismic Damage Assessment) project, which engaged high school students from North-East Italy in collecting data on buildings that were either unavailable from conventional exposure data sources or not easily retrievable via remote sensing techniques (Scaini et al., 2022).

To this end, we are developing a complex multimedia information system via web platform designed to collect, process, store, and distribute information to different knowledge users (policymakers, territorial planners, citizens) with targeted visualization strategies. The crowdsourcing initiatives are taking place in selected municipalities of Tuscany and Friuli regions (Italy), exposed to different natural hazards, such as earthquakes, tsunamis and landslides.  An online questionnaire has been created to assist the user in building data collection and minimize input errors. Simultaneously, building data, along with their photos, are stored in a structured database for research purposes.  For instance, building data and images are used as learning set to train a machine learning algorithm to identify specific features such as roof type, number of floors, and the presence of a basement. These algorithms can then be included in the online questionnaire to facilitate further data collection by automatically suggesting features associated to the buildings. A dedicated visualization tool is being developed on the web platform to showcase the effectiveness of this method in recognition of building features. We will demonstrate the data visualization tools developed on the web platform so far, highlighting the key features of the available exposure databases. The web platform is designed to provide an easy-to-use tool for communicating with various knowledge users, while also enhancing disaster awareness and preparedness, which is attained exploring and collecting data on the built environment.

This study is a contribution to the ongoing PRIN 2022 PNRR project SMILE “Statistical Machine Learning for Exposure development” (code P202247PK9, CUP B53D23029430001) within the European Union-NextGenerationEU program.

How to cite: Artese, M. T., Varini, E., Gagliardi, I., Ciocca, G., Piccoli, F., Rota, C., Del Soldato, M., Bianchini, S., Scaini, C., Peresan, A., and Brondi, P.: A web platform for crowdsourced collection, processing, and visualization of exposure data on buildings, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18225, https://doi.org/10.5194/egusphere-egu25-18225, 2025.

EGU25-21907 | Orals | NH4.4

Seismo-electromagnetism: observations and mechanisms 

Qinghua Huang

Seismogenic mechanism of strong earthquakes plays a fundamental role in disaster prevention. Electromagnetic methods, which are sensitive to fluid, have been widely adopted in the study on seismogenic structure and earthquake physics. Due to the increasing environmental disturbances and limited understanding on electromagnetic anomalies, electromagnetic data cannot fully show their potential values in disaster prevention. We propose an integrated work on seismogenic structure, identification of electromagnetic disturbances, and mechanism of seismo-electromagnetic anomalies. Based on the tests of synthetic and field data, we demonstrate that the multiple electromagnetic methods can reveal the feature of the multi-scaled seismogenic structure. With the developments of the new methodology based on deep learning and the seismo-electromagnetic coupling model, one can investigate the spatio-temporal characteristics of electromagnetic anomalies and their possible relationship with earthquakes. This study may contribute to the study on earthquake forecast and disaster prevention.

How to cite: Huang, Q.: Seismo-electromagnetism: observations and mechanisms, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21907, https://doi.org/10.5194/egusphere-egu25-21907, 2025.

Statistical models are a frequently used tool in hydrology, especially when it comes to estimating design floods, i.e. flood events that used to design flood protection systems or reservoirs. The often complex hydrological data, which are affected by e.g. missing values, extremes or time-varying processes, require sophisticated statistical models that take these challenges into account. As a scientist, developing such models can be a lot of fun and provide interesting insights. After months of thinking about the best model under certain statistical assumptions, proving asymptotic theorems and testing the model with synthetic data, you are happy and proud to have developed a new model. This model will hopefully be widely used in future research. The next step is to apply the model to a large real data set. The results look good on average. The results will be shared with practitioners, because of course you want the model to be useful for science and practice. And then: the phone call. You are told that your results are not plausible for a certain catchment area. And in general, the new model is not needed in practice because there is an established model. This example describes such a case and discusses ways of dealing with it. It is intended to illustrate the importance of communication between science and practice and a general understanding between both sides.

How to cite: Fischer, S.: When practical considerations impact your scientific model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1620, https://doi.org/10.5194/egusphere-egu25-1620, 2025.

EGU25-1660 | Orals | EOS4.8

The Minkowski–Bouligand dimension of a clay brick 

Nick van de Giesen and John Selker

In the early 1990's, fractals and chaos were hot. In 1987, James Gleick had published "Chaos: Making a New Science", popularizing non-linear dynamics. Hydrologists played an important role in the development of fractal theory. Hurst had discovered that sequences of dry and wet years for the Nile showed very long memory effects. Instead of the chance of a dry year following a dry year being 50%, Hurst found that there were surprisingly many long series of dry or wet years. Seven fat years, seven lean years, as it is noted in Genesis. Scott Tyler found fractals in soils ("Fractal processes in soil water retention"). At Cornell, where we were at the time, David Turcotte described "Fractals in geology and geophysics". A few years later, Ignacio Rodríguez-Iturbe and Andrea Rinaldo would publish "Fractal River Basins: Chance and Self-Organization". In short, fractals were exciting scientific gold.

A fractal is not just an obscure mathematical object but something that can actually be found everywhere in nature. Early on, a paper was published in Nature with the title "Fractal viscous fingering in clay slurries" by Van Damme, Obrecht, Levitz, Gatineau, and Laroche. They "only" did an experiment on a fractal embedded in 2D; we should be able to do one better and find the fractal dimension of the surface of cracking clay embedded in 3D. So out we went, collected some clay, mixed it with water in a cement mixer, siliconed together a shallow "aquarium", and poured in the slurry. To observe the cracking of the drying slurry, a video camera was mounted above the experiment, looking down and taking time-lapse images. To access the views from the sides, mirrors were installed at 45 degrees at each of the four sides. Lights made sure the camera captured high quality images. The whole set-up was enclosed in a frame with dark cloth to ensure that lighting was always the same.  We already had some box-counting code ready to calculate the fractal dimension of the surface, called the Minkowski–Bouligand dimension. One variable needed some extra attention, namely the boundary between the clay slurry and the glass sides. If the clay would cling to the sides, it would be difficult to understand the effects that this boundary condition had on the outcome of the experiment. Moreover, the cracks may not have become visible in the mirrors when the sides were covered with mud. So, instead, it was decided to make the sides hydrophobic with some mineral oil. This ensured that when the clay would start to shrink, it would come loose from the sides. Now, all we had to do was wait. It took only a week or so before the consolidated slurry started to shrink and to come loose from the sides. After that, the clay continued shrink for many weeks. This is how we learned that the fractal dimension of a shrinking brick of clay is (very close) to 3.0. 

How to cite: van de Giesen, N. and Selker, J.: The Minkowski–Bouligand dimension of a clay brick, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1660, https://doi.org/10.5194/egusphere-egu25-1660, 2025.

EGU25-5035 | Orals | EOS4.8

Landslides and hillslope erosion increase relief 

Stefan Hergarten and Jörg Robl

In 2018, we found exciting new results in landform evolution modeling by coupling the two simplest models of fluvial erosion and hillslope processes. While the stream-power incision model is the simplest model for detachment-limited fluvial erosion, the diffusion equation is the simplest description of hillslope processes at long timescales. Both processes were added at each grid cell without an explicit separation between channels and hillslopes because fluvial erosion automatically becomes dominant at large catchment sizes and negligible at small catchment sizes.

We found that increasing diffusion reduces the relief at small scales (individual hillslopes), but even increases the large-scale relief (entire catchments). As an immediate effect, the hillslopes become less steep. In turn, however, we observed that the network of the clearly incised valleys, which indicates dominance of fluvial erosion over diffusion, became smaller. So a smaller set of fluvially dominated grid cells had to erode the material entering from the hillslopes. To maintain a morphological equilibrium with a given uplift rate, the rivers had to steepen over long time. This steepening even overcompensated the immediate decrease in relief of the hillslopes.

This result was counterintuitive at first, but we were happy to find a reasonable explanation. So we even prepared a short manuscript for a prestigious  journal. We just did not submit it because we wanted to explain the effect quantitatively from the physical parameters of the model. From these theoretical considerations, we found that our numerical results did not only depend on the model parameters, but also on the spatial resolution of the model and noticed that this scaling problem was already discussed in a few published studies. Beyond the scaling problem, we also realized that applying the concept of detachment-limited fluvial erosion to the sediment brought from the hillslopes into the rivers is quite unrealistic. A later study including fluvial sediment transport and a model for hillslope processes that avoids scaling problems did not predict any increase in large-scale relief. So we finally realized that our original findings were mainly the result of a specific combination of models that should not be coupled this way and are not  as relevant for landform evolution as we thought.

This example illustrates many of the pitfalls of numerical modeling beyond purely technical issues. In particular, combining models that are widely used and make sense individually may still cause unexpected problems.

 

How to cite: Hergarten, S. and Robl, J.: Landslides and hillslope erosion increase relief, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5035, https://doi.org/10.5194/egusphere-egu25-5035, 2025.

EGU25-5091 | ECS | Orals | EOS4.8

(Re)(De)bugging tragedies with Hector 

Guillemette Legrand

In this presentation, I will discuss my research into the simple climate model Hector, which calculates temperature change based on the impact of various climate scenarios. More specifically, I will discuss how an artistic-led approach through (un)voluntary-caused computational bugs can help document the model's logic and socio-political implications. I will describe methods for collective 'debugging' to produce transdisciplinary knowledge (beyond solely scientific inquiry) to foster conversation about the potential and limits of current climate infrastructure to foster concrete climate actions. This research investigates the field of climate science through artistic practice, software and infrastructure studies, and participatory methods. To expand on the role of bugs in my investigation, I will elaborate on concrete examples of differences in perception of 'error' in the fields of arts and science, looking at case studies where mistakes or glitches have been valorised and mobilised through artistic practice to grapple with, appropriate, and/or repurpose scientific instruments.

How to cite: Legrand, G.: (Re)(De)bugging tragedies with Hector, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5091, https://doi.org/10.5194/egusphere-egu25-5091, 2025.

EGU25-5951 * | Orals | EOS4.8 | Highlight

Improving extreme temperature definitions until they are wrong 

Lukas Brunner, Maximilian Meindl, and Aiko Voigt

"Doesn't this look a bit strange?" 

It began with an innocent question during one of our Master's colloquia. And it could have ended there. "We were just following an approach from the literature". And who could argue against following the literature?

But it bugged me. During a long train ride, I began to think about the issue again. 10 hours and many papers later, I was only more confused: was it really that obvious, and why had no one picked up on it before? But sometimes the most obvious things are the most wicked, and after a few conversations with knowledgeable colleagues, I was sure we were in for an unexpected surprise. 

A commonly used approach to defining heat extremes is as exceedances of percentile-based thresholds that follow the seasonal cycle. Such relative extremes are then expected to be evenly distributed throughout the year. For example, over the 30-year period 1961-1990, we expect three (or 10%) of January 1s to exceed a 90th percentile threshold defined for the same period - and the same for all other days of the year. In a recent study, we show that there are many cases where this does not hold, not even close (Brunner and Voigt 2024).

Here, we tell the story of how this blunder spread in the literature out of the desire to improve extreme thresholds. We show that seemingly innocent changes can sometimes have unintended consequences and that taking the time to check the obvious can help avoid mistakes in science. 

 

Brunner L. and Voigt A. (2024): Pitfalls in diagnosing temperature extremes, Nature Communications, https://doi.org/10.1038/s41467-024-46349-x

How to cite: Brunner, L., Meindl, M., and Voigt, A.: Improving extreme temperature definitions until they are wrong, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5951, https://doi.org/10.5194/egusphere-egu25-5951, 2025.

When economists estimate the expected economic damages from current-day CO2 emissions, they usually calculate the social cost of carbon – that is, the aggregated damage caused by the emission of an additional ton of CO2. Several cost-benefit integrated assessment models (IAMs) are built to assess this quantity, and among them is the META model. This model is built specifically to assess the effects of tipping points on the social cost of carbon, and it usually operates stochastically. When integrating a deterministic, but small carbon cycle tipping point into the model, however, the social cost of carbon seems to explode: a few gigatons of additional emissions almost double the impact estimates of CO2 emissions! Well, maybe. In fact, these results are a pure artifact of two things: 1) the way in which social cost of carbon estimates are calculated with IAMs; and 2) the way that tipping points are implemented in the META model. And, of course, 3): a lack of initial thoughtfulness on behalf of myself. A thorough look into this issue shows that, as expected, a marginal change in emissions leads to a marginal change in damage estimates. While that result is rather boring, the previous blunder can actually be instructive about the scarcely-known methods used to obtain economic impact estimates of climate change.

How to cite: Schaumann, F.: Drastic increase in economic damages caused by a marginal increase in CO2 emissions?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9145, https://doi.org/10.5194/egusphere-egu25-9145, 2025.

EGU25-10285 | ECS | Orals | EOS4.8

How robust are modeled non-local temperature effects of historical land use changes really? 

Felix Jäger, Petra Sieber, Isla Simpson, David Lawrence, Peter Lawrence, and Sonia I. Seneviratne

Historically, large areas across the globe have been affected by deforestation or irrigation expansion. The replacement of forests with agricultural land and increased water availability in irrigated croplands altered the land’s surface properties, leading to influences of biogeophysical changes on near-surface temperature. From limited observations and mostly idealized simulations, we know that sufficiently large alterations of land surface properties can theoretically lead to systematic temperature and precipitation changes outside and even far from the altered areas. Not only the advection of temperature anomalies, but also changes in circulation and ocean feedbacks have been shown to be potential drivers of such non-local responses in single and multi-model studies.

We tested the robustness of non-local temperature signals to internal variability in the fully coupled Community Earth System Model 2 (CESM2) simulations of the historical period (1850 – 2014) with all forcings vs. all-but-land-use-change forcings. Doing so, we first found seemingly robust non-local temperature effects of land use change on the global and regional scale. But when accounting for the sampling of internal variability in the model using a large initial condition ensemble, the global scale signal was found to be indistinguishable from noise. Only regionally in some hotspots, we found robust and historically important non-local temperature signals. Through increasingly rigorous analysis, we reached a partly negative and unexpected but important finding, which may have implications for future assessments of comparably weak or spatially heterogeneous forcings to the Earth system.

How to cite: Jäger, F., Sieber, P., Simpson, I., Lawrence, D., Lawrence, P., and Seneviratne, S. I.: How robust are modeled non-local temperature effects of historical land use changes really?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10285, https://doi.org/10.5194/egusphere-egu25-10285, 2025.

EGU25-10615 | Orals | EOS4.8

Think twice – pitfalls in hydrological modelling 

Jan Seibert, Franziska Clerc-Schwarzenbach, Ilja van Meerveld, and Marc Vis

Failures are only common in science, and hydrological modelling is no exception. However, we modellers usually do not like to talk about our mistakes or our overly optimistic expectations and, thus, “negative” results usually do not get published. While there are examples where model failures indicated issues with the observational data, in this presentation the focus is on modelling studies, where some more (realistic) thinking could have helped to avoid disappointments. Examples include the unnecessary comparison of numerically identical model variants, naively optimistic expectations about increasing the physical basis of bucket-type models and excessively hopeful assumptions about the value of data.

How to cite: Seibert, J., Clerc-Schwarzenbach, F., van Meerveld, I., and Vis, M.: Think twice – pitfalls in hydrological modelling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10615, https://doi.org/10.5194/egusphere-egu25-10615, 2025.

EGU25-11357 | Orals | EOS4.8

Two steps forward, one step back: four years of progress and setbacks on invisible ship tracks 

Peter Manshausen, Anna Tippett, Edward Gryspeerdt, and Philip Stier

The idea of invisible ship tracks for the study of aerosol-cloud interactions sounds promising: We have been studying the effects of aerosols on clouds for many years, among others by investigating the bright lines of clouds left in low marine clouds by ships. However, only a small fraction of ships leaves behind visible tracks. This means we can only study aerosol-cloud interactions under certain meteorological conditions, biasing our understanding. Instead, by studying all clouds polluted by ships ('invisible ship tracks') with a methodology we developed, we should be able to get a full picture of aerosol-cloud interactions. A number of interesting and impactful results have come out of this research, along with several setbacks and corrections to initial results. Here, we examine them in order, showing how correcting for one identified bias can introduce two new ones. Unexpected glitches arise from sources as varied as: choices regarding ship track definition, retrieval geometry, specific weather systems biasing results, and mathematical subtleties. What can we conclude after four years of progress on this methodology? While some results still stand, others had to be significantly corrected. This makes us see invisible ship tracks as an example of research that is closer to a method of 'tinkering' than to a 'magnificent discovery'.

How to cite: Manshausen, P., Tippett, A., Gryspeerdt, E., and Stier, P.: Two steps forward, one step back: four years of progress and setbacks on invisible ship tracks, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11357, https://doi.org/10.5194/egusphere-egu25-11357, 2025.

EGU25-12720 | ECS | Posters on site | EOS4.8

Physical understanding of bugs to improve the representation of the climate system   

Hans Segura, Cathy Hohenegger, Reiner Schnur, and Bjorn Stevens

Earth system models are important tools used to understand our climate system and project possible changes in our climate due to anthropogenic and natural forcings. Human errors can occur in the development of Earth System models, i.e., bugs, giving an unphysical representation of our climate. A way to identify and solve bugs is to apply physical concepts. Here, we present an experience that occurred in the development of the ICOsahedral Non-hydrostatic model (ICON) as a kilometer-scale Earth System model, in which physically understanding a bug in the surface energy budget fixed land precipitation. 

In a simulation of ICON, referred to as ICON-bug, precipitation over tropical land continuously decreased across the simulation. This led to a ratio of land-ocean precipitation in the tropics of less than 0.7, which, otherwise, should be more than 0.86. As part of the possible explanations, the surface energy budget over land was targeted as a culprit. This idea relies on the influence of the interaction between soil moisture, surface heat fluxes, and winds to generate circulation favoring precipitation over dry land surfaces (Hohenegger and Stevens 2018). Indeed, the surface energy budget over dry surfaces in the ICON-bug showed an error in sensible heat flux. The sensible heat flux transmitted to the atmosphere was 70% of what was calculated for the surface module. Fixing this error closed the surface energy budget and increased land precipitation over the tropics, leading to a ratio of land-ocean precipitation of 0.94, close to observations. 

How to cite: Segura, H., Hohenegger, C., Schnur, R., and Stevens, B.: Physical understanding of bugs to improve the representation of the climate system  , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12720, https://doi.org/10.5194/egusphere-egu25-12720, 2025.

Whenever you study a phenomenon of mm to a few cm-scale in the laboratory which involves an interface, the question of surface tension arises. Surface tension is due to the fact that molecules prefer to stay with their own kind. Therefore, the creation of an interface between two fluids requires energy, and this influences the dynamics around the interface.

Surface tension can be a blessing: it produces the round shape of rain drops or the nice bubble shapes of colorful liquid in a lava lamp. It allows objects with a higher density to float on a liquid (such as an insect on water, or a silicone plate on sugar syrup). It can generate flow up a capillary.

However, it can also be a curse in the case of thermal convection. Purely thermal convection  develops when a plane layer of fluid is heated from below and cooled from above. The engine of motion is the thermal buoyancy of the fluid. This is what is happening in a planetary mantle on scales of hundreds to thousands kilometers. This is also what is happening in a closed box in the laboratory. But as soon as an interface exists, either between an upper and a lower experimental mantle, or in the case of a free surface at the top of the fluid layer, surface tension effects can become important. For exemple, the variation of surface tension with temperature was responsible for the beautiful honey-comb patterns imaged by Benard (1901) in the first systematic study of thermal convection with a free-surface. Surface tension is also going to act against the initiation of subduction (which acts to break the surface). 

We shall review in this presentation the signatures of surface tension in a convective context, and the different ways to minimize and/or remove the effects of surface tension in convection experiments, such as using miscible liquids, or a layer of experimental « sticky air ».

How to cite: Davaille, A.: Analog studies of mantle convection: the curse of surface tension (or not) ?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15059, https://doi.org/10.5194/egusphere-egu25-15059, 2025.

EGU25-15457 | Orals | EOS4.8

The crux with variability: too much or too little 

Markus Weiler

In hydrology we measure and follow the water. What if there is too much or too little? It happens a lot. As a field hydrologist, I frequently have to determine the location of a measurement, the time to take the measurement, the location to set up a field experiment, or the amount of a tracer to inject to study a hydrological system. However, this is a very bumpy road, as variability is often not in favor of my decisions because the distribution is wider than expected, bimodal instead of unimodal, or the probability of an event is theoretically small, but still an extreme event occurs during our experiment. I will showcase some examples to demonstrate what I mean and what I experienced, as well as how frequently the PhD students or Postdocs have suffered as a result of my decisions or of the unexpected variability: Climatic variability resulted in a winter without snow, just as new sensors were already deployed. Or the winter snowpack was extremely high, preventing any work at high altitudes in the Alps until mid of July, thereby reducing our field season by half. An ecohydological study to observe the effects of drought in a forest with a rainout shelter was ineffective because it occurred during an extremely dry year, making the control just as dry as our drought treatment. The automatic water sampler was set-up to collect stream water samples, but it was washed away four weeks later by the 50-year flood. The calculated amount of artificial tracer was either way too low, because the transit times of the system were much longer than expected, or it was far too high, resulting in colored streams or samples that had to be diluted by a factor of 100 due to much faster transit times Finally, and most expensively, we installed many trenches along forest roads to measure subsurface stormflow but after three years, we abandoned the measurements because we never measured a drop of water coming out of the trenches, as the bedrock permeability was much higher due to many high permeable fissures that prevented the formation of subsurface stormflow.  These experiments or observations failed because of unexpected variability in input, system properties or a lack of technical variability in the equipment. I will reflect on residual risk of failure in fieldwork related to that crux and discus approaches to reduce this risk.

How to cite: Weiler, M.: The crux with variability: too much or too little, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15457, https://doi.org/10.5194/egusphere-egu25-15457, 2025.

EGU25-15826 | ECS | Posters on site | EOS4.8

Output regridding can lead to Moiré pattern in km-scale global climate model data from ICON 

Benjamin Poschlod, Lukas Brunner, Benjamin Blanz, and Lukas Kluft

The emergence of global km-scale climate models allows us to study Earth's climate and its changes with unprecedented local detail. However, this step change in spatial resolution to grid spacings of 10 km or less also brings new challenges to the numerical methods used in the models, the storage of model output, and the processing of the output data into actionable climate information. The latest versions of the ICON-Sapphire model developed in the frame of the NextGEMS project address these challenges by running on an icosahedral grid while outputting data on the so-called HEALPix grid. Both grids are unstructured grids, which avoids, for example, the issue of longitude convergence. In addition, HEALPix allows data to be stored in a hierarchy of resolutions at different discrete zoom levels, making it easier for users to handle the data.  

The transition from the native 10 km grid to the output grid is made by a simple but very fast nearest-neighbour remapping. An advantage of this simple remapping approach is that the output fields are not distorted, i.e. the atmospheric states in the output remain self-consistent. As HEALPix only provides discrete zoom levels in the setup of the run, it was decided to remap to the closest available resolution of 12 km rather than to the next finer resolution of 6 km. This decision was made to avoid artificially increasing the number of grid points and to avoid creating duplicates through the nearest neighbour remapping.

As a consequence of this approach, wave-like patterns can emerge due to the Moiré effect that can result from the interaction of two grids. We find these patterns when looking at certain derived precipitation extremes, such as the annual maximum daily precipitation, the 10-year return level of hourly precipitation, or the frequency of dry days. At first, we interpreted these patterns as a plotting issue, as the figures might have too low resolution to cope with the high-resolution global plot (aliasing) leading to a Moiré pattern.

However, zooming in on the affected regions and closer examination of the data revealed that the pattern is in fact in the data. Further investigation with synthetic data confirmed the suspicion that the Moiré pattern was indeed caused by the remapping of the native 10 km icosahedral grid to the slightly coarser 12 km HEALPix grid. We hypothesise that precipitation is particularly affected by this issue, as it typically contains many grid cells with zero precipitation, with local clusters of non-zero values at the 15-minutely output interval. Yet, we cannot exclude the possibility that other variables are also affected.

As a consequence, if remapping is required, it is recommended to first remap from the native resolution to a finer resolution grid. As a next step, the conservative nature of the HEALPix hierarchy can be used to compute the coarser level. In this way it is likely to be possible to avoid aliasing and still keep the amount of output data the same.

How to cite: Poschlod, B., Brunner, L., Blanz, B., and Kluft, L.: Output regridding can lead to Moiré pattern in km-scale global climate model data from ICON, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15826, https://doi.org/10.5194/egusphere-egu25-15826, 2025.

EGU25-17676 | ECS | Posters on site | EOS4.8

What river plastic hotspots do not have in common 

Rahel Hauk, Adriaan J. Teuling, Tim H.M. van Emmerik, and Martine van der Ploeg

Plastic pollution is a global issue, across all environmental compartments. Rivers connect the terrestrial with the marine environment, and they transport various materials, among these plastic pollution. Rivers not only transport plastic, but also accumulate and store it, especially on riverbanks. In fact, plastic deposition and accumulation on riverbanks is a common occurrence. However, our understanding of why plastic is deposited on a certain riverbank is rather limited. Riverbanks along all major Dutch rivers have been monitored for plastic and other litter twice a year by citizen scientists, in some locations since 2018. This provides an extensive dataset on plastic accumulation, and we used these data with the aim of understanding the factors determining plastic concentration/accumulation variability over time and space. We tested multiple riverbank characteristics, such as vegetation, riverbank slope, population density, etc., hypothesized to be related to plastic litter. After having exhausted a long list of auxiliary data and analysis strategies, we found no significant results. Ultimately, we had a close look at ten consistent hotspots of macroplastic litter, along the Meuse, and Waal river. And once again, they seem to have nothing in common. But, there is a pattern, because some riverbanks have consistently very high densities of plastic litter so it does not seem completely random. We have been looking to explain spatial variability, whereas we might have to look at temporal consistency, and we shall not give up our efforts to bring order to this chaos.

How to cite: Hauk, R., Teuling, A. J., van Emmerik, T. H. M., and van der Ploeg, M.: What river plastic hotspots do not have in common, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17676, https://doi.org/10.5194/egusphere-egu25-17676, 2025.

EGU25-17811 | Posters on site | EOS4.8

Temporal variation of ambient noise at the Grande Dixence reservoir recorded by a nodal deployment 

Mita Uthaman, Laura Ermert, Angel Ling, Jonas Junker, Cinzia Ghisleni, and Anne Obermann

Grande Dixence, the tallest gravity dam in the world, is located in the Swiss Alps on the Dixence River with a catchment area of 4 km2 at a towering elevation of 2000m. The lake serves as a collecting point of melt water from 35 glaciers and reaches full capacity by late September, subsequently draining during winter and dropping to lowest levels in April. For a reservoir as large as the Grande Dixence, the variation in hydrological load can be expected to induce changes in crustal stress. The goal of this study was to harness the loading effect of the time-varying level of reservoir load as a source of known stress to investigate the variation in seismic velocity of the bedrock due to changes induced in crustal stress and strain rates. 22 seismic nodes were thus deployed along the banks of the reservoir which were operational from mid-August to mid-September, corresponding to the time period when the lake level reaches its maximum. Of the 22 nodes, 18 were deployed in closely spaced patches of six in order to carry out coherent stacking and to increase the signal-to-noise ratio, besides one group of three nodes and one single node. Measurement quality appears satisfactory: small local earthquakes are recorded well, and the probabilistic power spectral densities (PPSDs) computed for data quality validation evidence the ambient noise levels to be well within the global noise limits. However, the recorded noise is unexpectedly complex and, at periods shorter than 1 second, varies strongly by location. The 0.5--5s (0.2--2 Hz) period band at lakes generally records a diurnally varying noise level, often associated with lake generated microseism. Diurnal variations around 1 second of period are observed in our study as well. The amplitude of ambient noise level around 1 second of period is observed to be highest when the lake level changes, along with the prominent diurnal variation. A similar variation is observed in the seismic velocity variation (dv/v) computed from cross-correlated and auto-correlated ambient noise filtered between 0.5--1 Hz, with dv/v exhibiting a drop with rising lake level. These results provide preliminary evidence for possible change in crustal stress state with changing hydrological load. Future direction of this study consists of analytically modeling the results to quantify the influence of thermobarometric parameters on PPSDs and dv/v, and deconvolve it from the lake induced variations.

How to cite: Uthaman, M., Ermert, L., Ling, A., Junker, J., Ghisleni, C., and Obermann, A.: Temporal variation of ambient noise at the Grande Dixence reservoir recorded by a nodal deployment, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17811, https://doi.org/10.5194/egusphere-egu25-17811, 2025.

EGU25-18185 | Orals | EOS4.8

Advancing river plastic research through serendipity and stupidity 

Tim van Emmerik and the WUR-HWM River Plastic Team

Rivers play an important role in the global distribution of plastic pollution throughout the geosphere. Quantifying and understanding river plastic pollution is still an emerging field, which has advanced considerably thanks to broad efforts from science, practice, and society. Much progress in this field has been achieved through learning from failures, negative results, and unexpected outcomes. In this presentation we will provide several examples of serendipity and stupidity that has led to new insights, theories, methods, and completely new research lines. We will share what we learned from rivers flowing in the wrong direction, sensors that disappear, equipment blocked by invasive plants, and dealing with suspicious local authorities. Pushing the science sometimes requires an opportunistic approach, embracing surprises and chaos you may face along the way.

How to cite: van Emmerik, T. and the WUR-HWM River Plastic Team: Advancing river plastic research through serendipity and stupidity, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18185, https://doi.org/10.5194/egusphere-egu25-18185, 2025.

With the advent of parallel programming in the late 1990s. A port of the than available Max Planck Institutes for Meteorology spectral atmospheric model echam5 to MPI and OpenMP was done. For testing and validation of the hybrid parallelization a coherence algorithm was developed. The implementation has been incorporated into todays NWP and climate model ICON as well. The coherence algoritm consists of several stages: first one MPI rank is running the serial model against an n-task MPI parallelized model. During runtime the state vector is checked for binary-identity. If successfull a m-task MPI version can be compared to an m-task MPI version for high processor counts. The same schema can be used OpenMP parallelization. ONe MPI task runs the model serial using one OpenMP thread and a second MPI task runs k OpenMP threads. Again, the results are compared for binary-identity. As the testing needs to be done automatically, bit-identity is important for testing not necessarily for production.

The tesing revealed plenty of problems during the initial parallelization work of echam5 and showed constant appearing problems in the ICON development phase.

However, far in a couple of century long simulation the bit-identity was just by accident found to be broken: the search of the cause started!

How to cite: Kornblueh, L.: MPI and OpenMP coherence testing and vaildation: the hybris of testing non-deterministic model code, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18400, https://doi.org/10.5194/egusphere-egu25-18400, 2025.

EGU25-18981 | ECS | Posters on site | EOS4.8

Publishing BUGS: Insights from the Journal of Trial and Error 

Stefan Gaillard

Addressing positive publication bias and clearing out the file drawer has been at the core of the Journal of Trial and Error since its conception. Publishing the trial-and-error components of science is advantageous in numerous ways, as already pointed out in the description of this panel: errors can lead to unexpected insights and warning others about dead ends can prevent wasted time and other resources. Besides those advantages, publishing negative and null results facilitates conducting robust meta-analyses. In addition, predictive machine learning models benefit from training on data from all types of research rather than just data from studies with positive, exciting results; already researchers are reporting that models trained on published data are overly optimistic.

Besides publishing negative and null results as well as methodological failures, the Journal of Trial and Error couples each published study with a reflection article. The purpose of these reflection articles is to have a philosopher, sociologist or domain expert reflect on what exactly went wrong. This helps contextualize the failure, helping to pinpoint the systematic factors at play as well as helping the authors and other scientists to draw lessons from the reported research struggles which can be applied to improve future research.

Publishing failure brings with it some practical challenges: convincing authors to submit manuscripts detailing their trial-and-error; instructing peer reviewers on how to conduct peer review for the types of articles; differentiating between interesting … and uninformative, sloppy science; and determining the best formats to publish various failure-related outcomes in. Authors are still hesitant to publish their research struggles due to reputational concerns and time constraints. In addition, authors often fear that peer reviewers will be more critical of articles describing research failures compared to articles reporting positive results. To counteract this (perceived) tendency of peer reviewers to be more critical of research without positive results, we provide specific instructions to peer reviewers to only assess the quality of the study without taking into account the outcome. This then also ensures that we only publish research that adheres to the standards of the field rather than sloppy science. Whether submitted research provides informative insights is assed by the editor-in-chief and the handling editor.

Finally, we are constantly evaluating and innovating the types of articles we publish. Various types of errors and failures benefit from differing ways of reporting. For example, recently we introduced serendipity anecdotes, a format where scientists can anecdotally describe instances serendipity which occurred during their research. This format allows researchers to focus on the conditions which allowed for the serendipitous discovery rather than the research itself.    

How to cite: Gaillard, S.: Publishing BUGS: Insights from the Journal of Trial and Error, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18981, https://doi.org/10.5194/egusphere-egu25-18981, 2025.

It is common to perform two-dimensional simulations of mantle convection in spherical geometry. These have commonly been performed in axisymmetric geometry, i.e. (r, theta) coordinates, but subsequently we (Hernlund and Tackley, PEPI 2008) proposed using (r, phi) spherical annulus geometry and demonstrated its usefulness for low-viscosity-contrast calculations. 

When performing scaling studies in this geometry, however, strange results that did not match what is expected from Cartesian-geometry calculations were obtained when high-viscosity features (such as slabs) were present. It turns out that this is because the geometrical restriction forces deformation that is not present in 3 dimensions. Specifically, in a 2-D spherical approximation, a downwelling is forced to contract in the plane-perpendicular direction, requiring it to extend in the two in-plane directions. In other words, it is "squeezed" in the plane-perpendicular direction.  If the downwelling has a high viscosity, as a cold slab does, then it resists this forced deformation, sinking much more slowly than in three dimensions, in which it could sink with no deformation. This can cause unrealistic behaviour and scaling relationships for high viscosity contrasts. 

This problem can be solved by subtracting the geometrically-forced deformation ("squeezing") from the strain-rate tensor when calculating the stress tensor. Specifically, components of in-plane and plane-normal strain rate that are required by and proportional to the vertical (radial) velocity are subtracted, a procedure that is here termed "anti-squeeze". It is demonstrated here that this "anti-squeeze" correction results in sinking rates and scaling relationships that are similar to those in 3-D geometry whereas without it, abnormal and physically unrealistic results can be obtained for high viscosity contrasts. This correction has been used for 2-D geometries in the code StagYY (Tackley, PEPI 2008; Hernlund and Tackley, PEPI 2008) since 2010.

How to cite: Tackley, P.:  Adventures in Modelling Mantle Convection in a Two-Dimensional Spherical Annulus and Discovering the Need for "Anti-Squeeze”, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19890, https://doi.org/10.5194/egusphere-egu25-19890, 2025.

EGU25-20057 | Posters on site | EOS4.8

Some Perfectly Reasonable Ideas that Didn’t Work: Snow Hydrology 

Ross Woods

The science question: how can we use hydrological process knowledge to understand the timing and magnitude of seasonal streamflow in snow-influenced catchments.

What was known: in general, catchments with colder climates have later and larger seasonal streamflow peaks, because more snow tends to accumulate in colder catchments, and it melts later because the time when melt can occur is later in the year in colder climates. Numerical models with fine space and time resolution were able to resolve these phenomena, but there was no theory which directly linked long term climate to seasonal streamflow.

In 2009 I published a very simple deterministic theory of snow pack evolution. I tested it against snow observations at 6 locations in the western USA and it apparently worked well (although I later discovered that I'd been lucky).

In 2015 I used the snowmelt derived from this deterministic theory to predict timing and magnitude of seasonal streamflow. It did poorly, and revealed untested assumptions in my theory. I tried making the theory slightly more complicated by considering within-catchment variation in climate. This did not help.

In 2016 I created a stochastic version of the theory (a weakness identified in 2015), and then also considered the within-catchment variation in climate. It did better at reproducing measured snow storage, but did not help in understanding seasonal streamflow.

My next step will be to consider all forms of liquid water input, i.e. not just snowmelt but also rainfall.

What survived: I will continue to use the stochastic version of the theory as it is clearly an improvement. I will continue to examine whether within-catchment climate variability is important, but it seems unlikely after two negative results. But whether introducing liquid water input will be sufficient, who can say? I will also try to examine in more detail how it is that the finely-resolved numerical models can do an adequate job, but the theory cannot - it is in this gap that the answer probably lies.  However the models are very complicated, and it is not easy to get a good understanding of exactly what they are doing, even though we know which equations the are implementing.

 

How to cite: Woods, R.: Some Perfectly Reasonable Ideas that Didn’t Work: Snow Hydrology, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20057, https://doi.org/10.5194/egusphere-egu25-20057, 2025.

EGU25-20866 | ECS | Posters on site | EOS4.8

A case for open communication of bugs in climate models 

Jan Gärtner, Ulrike Proske, Nils Brüggemann, Oliver Gutjahr, Helmuth Haak, Dian Putrasahan, and Karl-Hermann Wieners

Climate models are not only numerical representations of scientific understanding but also human-written software, inherently subject to coding errors. While these errors may appear minor, they can have significant and unforeseen effects on the outcomes of complex, coupled models. Despite existing robust testing and documentation practices in many modeling centers, bugs broader implications are underexplored in the climate science literature.

We investigate a sea ice bug in the coupled atmosphere-ocean-sea ice model ICON, tracing its origin, effects, and implications. The bug stemmed from an incorrectly set logical flag, which caused the ocean to bypass friction from sea ice, leading to unrealistic surface velocities, especially in the presence of ocean eddies. We introduce a concise and visual approach to communicating bugs and conceptualize this case as part of a novel class of resolution-dependent bugs - long-standing bugs that emerge during the transition to high-resolution models, where kilometer-scale features are resolved.

By documenting this case, we highlight the broader relevance of addressing bugs and advocate for universal adoption of transparent bug documentation practices. This documentation complements the robust workflows already employed by many modeling centers and ensures lessons from individual cases benefit the wider climate modeling community.

How to cite: Gärtner, J., Proske, U., Brüggemann, N., Gutjahr, O., Haak, H., Putrasahan, D., and Wieners, K.-H.: A case for open communication of bugs in climate models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20866, https://doi.org/10.5194/egusphere-egu25-20866, 2025.

Mineralization in the Limerick Basin, located in southwest Ireland, uniquely associates with volcanic rocks, unlike other mineralized zones in the Irish midlands, where mineral systems align with large-scale normal faults. To better visualize the subsurface structures influencing Limerick’s mineralization, we conducted 2D gravity inversion incorporating geological and petrophysical constraints.

Conventional methods of deterministic inversion involve adding a model norm term to the data misfit term in the objective function to regularize an ill-posed problem and obtain stable solutions. While previous studies on constrained deterministic inversion have modified the model norm to include prior information or constraints in geophysical inversion, the complex nature of geological priors makes encoding this information mathematically and computationally challenging. To tackle this problem, we implemented a deep generative model, specifically a conditional variational autoencoder (cVAE)-based inversion framework, to incorporate structural constraints derived from drill hole and petrophysical data.

Initially, we tested this framework on a synthetic case by training the cVAE on thousands of 2D density models comprising geological features analogous to the field geology and populated with density values consistent with the drill core measurements acquired from the study area. Artificial drill holes were created to fix the depths of geological units at the drill hole contact points across all training models, ensuring that the predicted models adhered to prior constraints. Following training, we tested the network on some test data, which showed that the predicted models successfully captured the structural and petrophysical property constraints. The geometries of the geological features were also well recovered.

We applied this method to gravity data from a NW-SE trending profile crossing the western part of Limerick Syncline. Thousands of density models were generated using drill hole data, incorporating measured rock densities for training. Since the profile’s central and deeper sections lacked sufficient geological data for direct validation of the results, we implemented a hypothesis-testing approach. In each hypothesis, geological features were added to the training density models based on prior geological knowledge of the study area. If simulated data from an inverted model failed to match field data, more geological features were added to the training models in the next hypothesis, and the workflow was repeated to achieve a low data misfit.

The inversion provided three key insights into the study area’s geology. First, it identified potential volcanic intrusions in the southern Limerick Syncline, possibly extending from depths below the basement. Second, it estimated the syncline’s geometry in areas with limited geological constraints. Third, it revealed a sharp vertical displacement in stratigraphy, indicating a potential south-dipping fault in the northwest portion of the syncline. This fault may have influenced mineralizing fluid migration, playing a critical role in mineral deposit localization.

How to cite: Chakraborti, P., Sun, J., and Melo, A.: An improved characterization of the subsurface in the Limerick Basin (Ireland) using deep generative model-based 2D gravity inversion constrained with drill hole and petrophysics data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-655, https://doi.org/10.5194/egusphere-egu25-655, 2025.

EGU25-700 | ECS | Posters on site | ERE4.1

Towards sustainable activity in artisanal gold mining in Hoggar 

Mouloud Issaad and Aboulyakdane Bakelli

The Algerian government issued many artisanal gold mining authorizations to formalize gold-bearing quartz vein mining within the Hoggar shield. However, as observed all-over the world, miners have no technical knowledge and not use basics prospecting tools during mining; generally, they don’t incorporate geology and mineralogy knowledge in mining practices. The objective of this study is to provide artisanal miners with recommendations to enhance the sustainability of their mining projects by employing rational and optimized exploitation methods. For this study, nine artisanal mine sites were selected within the Taskret gold field, at approximately 150 Km from eastern Tamanrasset. The ore deposits consist mainly of gold-bearing quartz veins hosted by metamorphic rocks. Firstly, we will conduct a comprehensive study of the mineralogy of run of mine (ROM) samples, including both ore and rocks, using X-ray diffraction (XRD). Thin and thick sections will be meticulously prepared from the rock fragments and ores, enabling us to determine mineralogy and textures through optical microscopy, scanning electron microscopy (SEM-EDX), and electron microprobe techniques. Gold grade determination will be performed using fire assay, while chemical characterization of other elements will be carried out through ICP-MS analyses. This holistic approach will provide us with vital insights into the geological and mineralogical characteristics of ROM materials, allowing us to make recommendations for enhancing the sustainability of artisanal mining practices in the Taskret gold field. Indeed, before any mining operations and ore treatment the good understanding of the ore mineralogy is very important to optimize the gold recovery and to minimize environmental impact of the activity. This project will significantly contribute to a rational and sustainable artisanal mining in Algeria, especially in the Hoggar, by giving scientific recommendation based on mineralogy of gold bearing minerals.

How to cite: Issaad, M. and Bakelli, A.: Towards sustainable activity in artisanal gold mining in Hoggar, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-700, https://doi.org/10.5194/egusphere-egu25-700, 2025.

EGU25-940 | ECS | Posters on site | ERE4.1

Design of MWPC-based muography measurements for geophysical research 

Boglárka Abigél Stefán, László Balázs, Gergő Hamar, Gergely Surányi, and Dezső Varga

 Muography is a most novel tool for geophysical density mapping. This
developing interdisciplinary research area is based on the detection of
muons originating from cosmic rays, allowing density-based non-destructive
investigations of the interior of objects up to the size of a mountain.
The cornerstone of the technology is that muons lose energy depending on
the density of the rock and the distance it travels through it. Thus, the
number and direction of the incoming muons can be used to determine
density anomalies (e.g. cavity, cave, ore) during data processing.


   Our Group in HUN-REN WignerRCP Budapest is internationally renowned in
the development of high-performance muon-detectors, data processing
procedures, and exploring new applications for muography.


   Recently we have developed a muographic-survey planning software, thus
for the various scenarios the optimal detector configuration and
orientations could be calculated.


   Reliability of this novel technology and any new equipments shall be
proven in well-known sites. The Jánossy Underground Laboratory (JURLab) in
Budapest is a simple-geometry multi-level underground infrastructure,
excellent for detector verifications and quantifying limits of underground
muographic surveys.

   We will present recent measurement series from JURLab campaigns;
validation of predicted yields with real data, and its implementation for
the tomographic inversion. Case studies and pilots from mining
applications will be shown.

How to cite: Stefán, B. A., Balázs, L., Hamar, G., Surányi, G., and Varga, D.: Design of MWPC-based muography measurements for geophysical research, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-940, https://doi.org/10.5194/egusphere-egu25-940, 2025.

EGU25-983 | ECS | Orals | ERE4.1

Muography: A novel method of density measurement for mining and surveying 

Bence Rábóczki, Gergely Surányi, Gergő Hamar, and László Balázs

Muography is a rapidly developing geophysical method, that utilises high energy cosmic muon particles to explore the inner structure of large objects, such as volcanoes, pyramids or mountains. Cosmic muons originate from upper atmosphere and have a known, steady, angle dependent flux on the surface. Muons are absorbed as they pass through matter, depending on the density of the material along their trajectories. By comparing the expected and the measured muon flux and using geoinformatic models of the observed area it is possibble to calculate the density distribution inside these structures. Our group at the HUN-REN Wigner RCP focuses on muographic imaging including research, hardware development and geophysical applications. There are several ongoing muographic projects inside European mines. Our measurements were able to confirm known density anomalies in these areas. The method can be applied to a wide variety of problems, such as determining the shape and density of geological formations or ore bodies, the location of caves or fractured zones located up to a few hundred meters underground. The presentation describes the priciples of muography and demonstrates it’s usability with examples from multiple projects.

How to cite: Rábóczki, B., Surányi, G., Hamar, G., and Balázs, L.: Muography: A novel method of density measurement for mining and surveying, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-983, https://doi.org/10.5194/egusphere-egu25-983, 2025.

EGU25-1258 | ECS | Posters on site | ERE4.1

Pollution monitoring at the Black Angel legacy mine in West Greenland using in-situ portable X-Ray Fluorescence (pXRF) measurements 

Christian Frigaard Rasmussen, Jens Søndergaard, Kristian Tommerup Vad, and Christian Juncher Jørgensen

In Greenland, mining has been undertaken in remote areas for more than 150 years and long before legislation for environmental protection was implemented. The Black Angel mine by the Affalikassaa fjord in Central West Greenland served as a marble quarry, known as Maarmorilik, operating in the 1930s when a metal-sulphide ore body was discovered in the ‘Black Angel’ mountain on the other side of the fjord. This discovery led to establishment of the Black Angel lead-zinc mine, operating from 1973-1990 with a total of 13.5 million tons of ore produced from an ore body located 600 meters up a vertical mountain side and only accessible via cable cart spanning 1500 meters across the fjord. Mining was done by the “Room-and-Pillar” method, where ore was crushed inside the mine before being transported via cable cart to the processing facility. Large amounts of pyrite and sphalerite bearing waste rock were dumped directly out of mine tunnel openings at approx. 600 meters altitude onto the steep mountain slopes below as well as and onto the “Tributary Glacier” towards the Greenland Ice Sheet. Since deposition, the waste rock has been exposed to the elements with significant leaching of heavy metals and dispersion of fine particles into the terrestrial and marine environments. Environmental monitoring since mine-closure in 1990 has documented a widespread pollution of Pb in the area. However, the knowledge on the geochemical composition of the different waste rock dumps, their relative contributions to both historical, current and future releases of heavy metals to the environment as well as future risk due to permafrost thaw and surface erosion is limited by a lack of widespread geochemical characterization of deposited waste rock.

In the current study we present the first large scale in-situ pollution monitoring at the legacy Black Angel mine, using portable X-Ray Fluorescence spectrometry (pXRF). pXRF has been shown to provide fast, accurate and cost-effective results for many heavy metals in sediment and soil, enabling effective in-situ identification of pollution hot-spots. Results from this study show significant variation in heavy metal content between different waste rock dump sites. The highest concentrations of Pb, Zn and Cd are found in the North Face Dump and 17xCut established early in the mine's history, and lower, yet still significant concentrations are found in the much younger Tributary Glacier dump. We find that the waste rock from the Tributary glacier has been reworked and transported downstream where we measure increased concentrations of heavy metals. This highlights the large environmental risks associated with depositing mine waste on dynamic landforms. Current surface and bank erosion of fine particles from waste rock dumps will likely continue in the future as a warmer climate may increase erosion potential in response to large precipitation events as well as changes in snow cover. The remaining environmental risk is generally dominated by the mine closure strategy of leaving waste rock exposed to the environment, with only limited impacts from future warming and thawing permafrost.

How to cite: Frigaard Rasmussen, C., Søndergaard, J., Tommerup Vad, K., and Juncher Jørgensen, C.: Pollution monitoring at the Black Angel legacy mine in West Greenland using in-situ portable X-Ray Fluorescence (pXRF) measurements, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1258, https://doi.org/10.5194/egusphere-egu25-1258, 2025.

EGU25-2011 | ECS | Orals | ERE4.1

Classification of Phosphate Sedimentary Facies and Estimation of Carbonate-Fluorapatite Abundance Using Hyperspectral Infrared Imaging 

Houda Lkhaoua, Otmane Raji, Abdellatif Elghali, Radouan El bamiki, Abdelhafid El alaoui el fels, and Mostafa Benzaazoua

Over recent years, the use of hyperspectral infrared imaging has significantly increased in the mining sector, offering numerous applications from geological exploration and mining to sorting and the rehabilitation. However, this technology remains underutilized in the phosphate mining industry, particularly in countries like Morocco, where phosphates represent over 70% of the world's reserves. In this study, the objective is to investigate the use of hyperspectral infrared imagery as a tool to identify and characterize sedimentary phosphate facies for automated facies core logging applications as well as to identify the spectral signature of Carbonate-Fluorapatite (CFA), the primary phosphate mineral phase in sedimentary phosphates, in order to estimate its abundance.To achieve this, six samples have been carefully selected from the Benguerir phosphate sequence to represent the commonly encountered indurated facies. The samples were scanned using a core scanner equipped with three hyperspectral sensors: a Visible Near-Infrared (VNIR) camera, a Short-Wavelength Infrared (SWIR) camera, and a Medium-Wavelength Infrared (MWIR) camera. The covered wavelength interval ranges from 0.4 µm to 5.3 µm, with spatial resolutions varying from 0.117 mm/pixel to 0.228 mm/pixel. Eight facies were identified in the studied samples and characterized through petrography and XRF geochemical analysis of the whole rock. Subsequently, a spectral library was established for each of these facies. Moreover, a sample area rich in CFA was selected and characterized by automated SEM using Tescan Integrated Mineral Analyzer (TIMA). The results indicate that all the facies exhibit distinguishable signatures in the various VNIR, SWIR, and MWIR intervals. However, the SWIR and MWIR intervals proves to be the most effective sensors for distinguishing these facies. The results indicate also that the Spectral Angle Mapper (SAM) is the most efficient method, achieving an overall accuracy of 98,75% in distinguishing the studied facies in the MWIR wavelength range. Additionally, several statistical methods were also tested to estimate the abundance of CFA using the spectral signature derived from the comparison between the SEM mineral maps and corresponding hyperspectral images. Band rationing (B(3.4µm)/B(4.7µm)) * (B(3.4µm)/B(3.9µm)) has demonstrated effective in identifying and estimating the abundance of CFA demonstrating the potential of hyperspectral imaging as a rapid and cost-effective method for the characterization of phosphates in terms of their apatite content.

How to cite: Lkhaoua, H., Raji, O., Elghali, A., El bamiki, R., El alaoui el fels, A., and Benzaazoua, M.: Classification of Phosphate Sedimentary Facies and Estimation of Carbonate-Fluorapatite Abundance Using Hyperspectral Infrared Imaging, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2011, https://doi.org/10.5194/egusphere-egu25-2011, 2025.

EGU25-2614 | Orals | ERE4.1

Rare Earth Elements – Multiphysics AI-aided Autonomous Prospecting (REE -MAP) 

Yuxin Wu, Chunwei Chou, JunWoo Chung, Baptiste Dafflon, Jim Panaro, Brian Quiter, Emil Rofors, Robin Tibaut, Jiannan Wang, Mike Whittaker, and John Wu

The growing demand for Rare Earth Elements and Critical Minerals (REE-CM) has heightened interest in extracting these elements from secondary resources, such as coal waste. Similar to traditional mining, resource mapping and prospecting to identify high concentration “hot zones” is key to prioritizing extraction efforts. Mapping REE-CM in unconventional sources is challenging due to low and variable concentrations and complex material characteristics. This study introduces an AI-aided, drone based multi-physics approach to rapidly characterize REE-CM hot zones in coal mine tailings. Our methodology integrates geophysical, radiological, hyperspectral and other technologies deployed on drones, complemented by other ground and laboratory analytical techniques. AI algorithms are key for integrating and interpreting complex multi-physics datasets to identify REE hot zones and optimize sensor selection and deployment. Field demonstrations at coal refuse and ash sites in Pennsylvania were carried out to validate the practical feasibility of this approach. The results revealed promising links between drone-acquired multi-physical signals and REE concentrations, and REE predictions with AI were validated with ground truth. Our study validated the feasibility of using drone-based multi-physics surveys to map REE concentrations in coal wastes to enhance their economic viability for recovery and guide extraction prioritization.

How to cite: Wu, Y., Chou, C., Chung, J., Dafflon, B., Panaro, J., Quiter, B., Rofors, E., Tibaut, R., Wang, J., Whittaker, M., and Wu, J.: Rare Earth Elements – Multiphysics AI-aided Autonomous Prospecting (REE -MAP), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2614, https://doi.org/10.5194/egusphere-egu25-2614, 2025.

EGU25-4279 | ECS | Orals | ERE4.1

Towards a Global Carbonatite Atlas: A Satellite Remote Sensing Approach to Mapping and Characterization  

Rupsa Chakraborty, René Booysen, Saeid Asadzadeh, Sam Thiele, and Richard Gloaguen

Rare Earth Elements (REEs) have become critical for global technological advancements and, consequently, economic growth. Ensuring supply requires significant future exploration, potentially including the use of space-borne hyperspectral data for direct mapping of REEs. While space-borne detection of REEs has been demonstrated (e.g., Asadzadeh et al., 2024), this approach has limited application. Low concentrations of these valuable resources in most carbonatite host rocks and small sizes of ore zones represent a  major hurdle and complicate reliable detection and mapping efforts. 

We propose a comprehensive approach to remotely characterise carbonatites, which are known to host REEs, with the aim of improving our overall understanding of these unusual rocks and better identifying potentially fertile systems. Carbonatites are typically classified into three types: calcio-carbonatites, magnesio-carbonatites, and ferro-carbonatites. However, recent studies, such as Mitchell & Gittins (2022), suggest additional variants that don't fit these categories, indicating the current classification system may require further refinement. Regardless of classification complexities, the composite mineralogical phases of carbonatites are spectrally active and exhibit distinctive absorption features in hyperspectral data. Furthermore, the presence of alteration halos and the structural controls commonly associated with carbonatite structures make these sites well-suited for optical remote sensing studies by both hyperspectral and multispectral datasets. This paves the way for the development of a global carbonatite atlas based on remote sensing data.

We demonstrate the feasibility of the approach using two REE-bearing carbonatite complexes in Namibia—Lofdal and Marinkas-Quellen. We selected EnMAP provided by the German Aerospace Center (DLR) hyperspectral data as they are the most accurate to this date (Chakraborty et,al., 2024). We employed different processing techniques such as minimum wavelength mapping and spectral abundance analysis to map the carbonatite lithologies in each of the two sites individually. We then streamlined the workflow to identify common parameters and trained a decision tree to map the broader carbonatite footprints across both sites. In parallel, Sentinel-2 multispectral data was used to map geological structures (e.g., dykes, faults, and bedding) aiming to understand controls on carbonatite emplacement. A fusion-based resolution enhancement algorithm was also applied to integrate EnMAP with Sentinel-2 data, providing a more spatially detailed understanding of the targets. 

We aim to expand this study to include a wider range of carbonatite complexes, with the goal of creating a global carbonatite atlas. By covering diverse geological settings and ages, this atlas will capture the full spectrum of mineralogical variation and structural features, enhancing our understanding of carbonatite bodies. This atlas not only will promote the applications of remote sensing techniques in carbonatite studies but also provide a valuable basis for future exploration of REEs in carbonatite settings. 

1. Asadzadeh, S., Koellner, N., & Chabrillat, S. (2024). Detecting rare earth elements using EnMAP hyperspectral satellite data: a case study from Mountain Pass, California. Scientific Reports

2. Mitchell, R. H., & Gittins, J. (2022). Carbonatites and carbothermalites: A revised classification. Lithos

3. Chakraborty, R., Rachdi, I., Thiele, S., Booysen, R., Kirsch, M., Lorenz, S., ... & Sebari, I. (2024). A Spectral and Spatial Comparison of Satellite-Based Hyperspectral Data for Geological Mapping. Remote Sensing

How to cite: Chakraborty, R., Booysen, R., Asadzadeh, S., Thiele, S., and Gloaguen, R.: Towards a Global Carbonatite Atlas: A Satellite Remote Sensing Approach to Mapping and Characterization , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4279, https://doi.org/10.5194/egusphere-egu25-4279, 2025.

EGU25-6028 | Posters on site | ERE4.1

 Evaluating LIBS analysis for improved steel alloy identification in end-of-life vehicle recycling  

Margret C. Fuchs, Rahul Patil, Aastha Singh, Gopi Regulan, Yuleika C. Madriz Diaz, Rene Ziegenrücker, and Richard Gloaguen

Securing raw material supply for high-tech products and reducing their ecological-economic footprint has become a pressing challenge for our society due to increasing demands while natural resources deplete. One solution is seen in closing material loops by recycling. But to ensure successful re-entry of secondary resources into the production chain essentially relies on the accurate identification of materials in mixed waste streams in order to allow for precise sorting into as pure as possible material types. A particular relevant, but at the same time particularly challenging, task relates to the identification of metal alloys. A wide variety has been engineered to provide highly specific functionalities of individual metals such as, for example, steel in the automotive industry. Innovation over many years resulted in cars containing multiple high-performance steel alloys. At their end-of-life, car recycling routines can sort out concentrates of steel, but mixing the different alloys prevents the recycling material from meeting the quality criteria needed for new car production, and hence, cause downcycling. Although several sensor-based sorting solutions are available to map qualitative material differences for many waste streams, a precise and quantitative solution is needed to differentiate between steel alloy types. LIBS provides a promising solution as it allows for elemental analysis along with concentration information in a fast and contact-free manner compatible with conveyor-belt operations.

            With this contribution, we highlight the challenges of steel alloy detection using LIBS and point out solutions for analytical workflows and practical applications. This involves especially the detailed investigation of measurement parameters, establishment of calibration models for most relevant elements and discuss potential influences from disturbances such as from surface coating. The results suggest a successful discrimination of automotive-relevant steel alloys. The workflow hence, provides the basis for improved alloy-specific sorting products. Providing such analytical tools and corresponding workflows will help for increasing the quality of recycling and reducing the risk of increasingly complex recycling mixtures after multiple cycles. In this context, accurate quantitative LIBS results provide one cornerstone to future innovations on material recycling by products that at least partially re-enter high-performance product cycles.

How to cite: Fuchs, M. C., Patil, R., Singh, A., Regulan, G., Madriz Diaz, Y. C., Ziegenrücker, R., and Gloaguen, R.:  Evaluating LIBS analysis for improved steel alloy identification in end-of-life vehicle recycling , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6028, https://doi.org/10.5194/egusphere-egu25-6028, 2025.

The environmental and social issues related to abandoned mines are prevalent worldwide. Each country has developed various chemical, physical, and biological mine reclamation technologies to address these challenges, and the results have primarily been published in papers or patents. Therefore, analyzing relevant papers and patents to understand the trends in the mine reclamation industry is essential. This study conducts a quantitative analysis of papers and patents related to mine reclamation technologies to identify the latest technological trends, address limitations, and propose future R&D development directions. Using Data Envelopment Analysis (DEA), this study evaluates the efficiency of diffusing papers and patents produced by national R&D investments in related industries, academia, research institutions, and government agencies. The input variables included the number of papers and patents, whereas the output variables comprised the number of citations for papers and patents and the number of triadic patent families. Using a comparative analysis of efficiency across countries, this study derives insights into the knowledge dissemination effects of research outcomes at the national level. To enhance knowledge dissemination and its impact in each country, research centered on solving current issues, improving data reliability, promoting multidisciplinary studies, and strengthening international cooperation is necessary. This study is significant as it provides future research directions for mine reclamation technologies and facilitates the application and commercialization of the developed technologies.

How to cite: Bae, S. W. and Bae, J.: Analysis of Knowledge Spillover Effects Using Data Envelopment Analysis on Papers and Patents Related to Mine Reclamation Technology, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7522, https://doi.org/10.5194/egusphere-egu25-7522, 2025.

EGU25-7554 | Posters on site | ERE4.1

Characteristics and Key Exploration Directions of Gold Deposits in China 

Bin Wang, Jingchao Li, and Jian Li

Based on the geodynamic environment, basic geological characteristics of minerals and so on, gold deposits in China are divided into 11 categories, of which tectonic fracture altered rock, mid-intrudes and contact zone, micro-fine disseminated and continental volcanic types are the main prospecting kinds. The metallogenic age of gold deposits in China is dominated by the Mesozoic and Cenozoic. According to the geotectonic units, geological evolution, geological conditions, spatial distribution, gold deposits types, metallogenic factors etc., 42 gold concentration areas are initially determined, and have a concentrated distribution feature. On the basis of the gold exploration density, gold concentration areas are divided into high, medium and low level areas. High ones are mainly distributed in the central and eastern regions. 93.04% of the gold exploration drillings are within 500 meters, but there are some problems such as less and shallower of drilling verification etc.. The paper discusses the resource potentials of gold deposits, and proposes the future prospecting directions and suggestions. The deep and periphery of old mines in the central and eastern regions and western area especially in Xinjiang and Qinghai will be the future key prospecting one, and have huge potential gold reserves. If the exploration depth is extended to 2,000 meters shallow, the gold resources will double. 

How to cite: Wang, B., Li, J., and Li, J.: Characteristics and Key Exploration Directions of Gold Deposits in China, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7554, https://doi.org/10.5194/egusphere-egu25-7554, 2025.

EGU25-7634 | Posters on site | ERE4.1

Study on the mineralogical and geochemical characteristics within sediments in southwestern Taiwan 

Yen-Hua Chen, Chien-Che Huang, and Han-Lin Yeh

Rare earth elements are important resources and they can be widely used in smart phones, electric vehicles, and smart home appliances, etc. Recently, countries around the world pay attentions to their own rare earth resources and set policies to cope with the country's future development. Therefore, rare earth resources have obviously become valuable strategic materials. Rare earth minerals are mainly occurred in placer depositions in Taiwan. The literature on rare earth resources in Taiwan is quite limited; there are only a few studies on the characteristics of heavy sand deposits, and only a few about the distribution of heavy minerals in southwestern Taiwan. Therefore, this study utilizes the drainage basin of Zengwun River (the upstream, midstream and downstream of the river) as the study site for rare earth resources in southwestern Taiwan. Using the sediments in the river and offshore as study samples, the systematic investigation on the properties of rare earth minerals in river sands and sea sands will be deeply studied. This study aims to investigate the relevant characteristics of rare earth resources (microstructure, types of rare earth minerals, and concentrations of rare earth elements, etc.) and to provide the comprehensive results pertaining to the potential placer rare earth ore in the drainage basin of Zengwun River of southwestern Taiwan. The XRD data indicated that the samples contained major minerals of quartz, feldspar, muscovite/illite, kaolinite, and chlorite; some minor minerals of rutile, calcite, and monazite (rare earth mineral). The SEM results showed that these monazites can be divided into detrital and aggregated monazites. The aggregated monazite presented two different occurrences. Type I aggregated monazite displayed a skeletal morphology associated with quartz and feldspar inclusions. Type II aggregated monazite was symbiotic with allanites or TiO2 polymorphs. The REE concentration in this study area will be evaluated and compared with the UCC average and active REE mining countries.

How to cite: Chen, Y.-H., Huang, C.-C., and Yeh, H.-L.: Study on the mineralogical and geochemical characteristics within sediments in southwestern Taiwan, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7634, https://doi.org/10.5194/egusphere-egu25-7634, 2025.

EGU25-7860 | ECS | Posters on site | ERE4.1

Distribution and controlling factors of cobalt in polymetallic nodules in the Philippine Sea 

Liwei Liu, Chunmei Dong, Wei Huang, Yong Zhang, and Jun Sun

         Deep-sea polymetallic nodules are rich in a variety of essential metals, among which Co, as a redox-sensitive element, is not only an indispensable core material in modern industry and science, but also an effective indicator for recording changes in the marine environment. The geochemical and mineralogical analyses carried out on typical polymetallic nodule samples from the Philippine Sea, combined with microzonation morphology and compositional tests. The results revealed that the samples from the study area have Mn/Fe ranging from 0.73 to 2.24, with an average of 1.20, and the nodules are hydrogenetic, formed mainly in an oxidizing environment, with Co mainly hosted within hydroxylated manganese ores.

          Compared with the Co-rich (>0.4%) aquatic-origin nodules from the western Pacific, the nodule samples from the study area have low Co content (0.06% to 0.25%) but slightly higher Si, Al and other detrital fractions (mean values of 9.21% and 4.79%). Based on the empirical formula of Co age, it is inferred that there is no significant break in the growth process of the nodule samples in the study area, which may be due to the relatively short duration of nodule growth in the region and the restricting influence of land-based component supply (wind and dust) on the further enrichment of Co during the growth process in the study area. The polymetallic nodules in the study area are predominantly distributed below the carbonate compensation depth (CCD), where high bottom water oxygen content, low sedimentation rates, and low organic matter content create favorable conditions for subsequent sustained enrichment and proliferation of Co in the nodules.

Keywords: Polymetallic nodule, Philippine Sea; Co; Controlling factors

How to cite: Liu, L., Dong, C., Huang, W., Zhang, Y., and Sun, J.: Distribution and controlling factors of cobalt in polymetallic nodules in the Philippine Sea, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7860, https://doi.org/10.5194/egusphere-egu25-7860, 2025.

EGU25-7895 | Posters on site | ERE4.1

Prediction of the abundance of ferromanganese nodules using Gaussian Process Regression based on multisource geological data in the western Pacific deep-sea basin 

Yong Yang, Hong Song, Shuang Hong, Xiaobing Li, Jiangbo Ren, Yonggang Liu, Miao Yu, and Gaowen He

Ferromanganese nodules, rich in cobalt (Co), nickel (Ni), copper (Cu), manganese (Mn), and rare earth elements (REEs), are important marine mineral resources with the utmost capacity for commercial employment in the future. Recently, the discovery of high abundant Co-rich nodules in the Western Pacific has attracted significant attention. The prediction of nodule abundance is a vital geological problem to be solved in marine mineral resource exploration. Based on the multisource geological data of the study area in the western Pacific Ocean acquired through acoustic, optic and geological sampling, a stochastic probabilistic prediction for nodule abundance was developed via Gaussian process regression (GPR). The results revealed that the predicted abundance of nodules ranged from 0 to 71.2 kg/m2, with an average abundance of 26.3 kg/m2. The high-abundance (~30.0 kg/m2) nodules are mainly distributed in the deep-sea basins around several seamounts, and they may be spatially coupled with the Co-rich crust distributed over seamounts in the targeted study area. Compared to traditional machine learning approaches, such as stepwise linear regression, regression trees and support vector machine, intelligent prediction of nodule abundance by GPR is achieved with improved accuracy. Moreover, with the predicted abundance, the prediction error is obtained simultaneously by GPR. The deep-sea basins between the Magallan and Marcus-Wake seamounts are considered potential areas for further exploration of Co-rich ferromanganese nodules in the western Pacific Ocean.

How to cite: Yang, Y., Song, H., Hong, S., Li, X., Ren, J., Liu, Y., Yu, M., and He, G.: Prediction of the abundance of ferromanganese nodules using Gaussian Process Regression based on multisource geological data in the western Pacific deep-sea basin, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7895, https://doi.org/10.5194/egusphere-egu25-7895, 2025.

EGU25-9451 | Orals | ERE4.1

Biogeochemical processes driving the fate of arsenic in phytostabilised mine tailings: elaboration of a conceptual model based on multi-scale experiments 

Fabienne Battaglia-Brunet, Hugues Thouin, Ulysse Moreau, Vincent Milesi, Catherine Joulian, Hafida Tris, Michael Charron, Louis De Lary de Latour, Nicolas Devau, Marina Le Guédard, Olivier Pible, and Lydie Le Forestier

Securing mine tailings represents a major environmental challenge. Metal mines frequently produce solid wastes containing iron (Fe) and sulfur (S), often associated with the toxic metalloid arsenic (As). Phytostabilisation often appears as a suitable option to decrease the dispersion of particles by erosion, at a moderate cost. However, site managers need a more comprehensive view of all the consequences linked to this remediation technique, notably the side effects on the other pathways controlling As and metals mobility out of the tailings. The present research aims to develop a tool for predicting the mobility and plant toxicity of As in and outside the assisted phytostabilised tailings dump, based on developing an innovative reactive transport model (RTM) explicitly integrating bacterially-catalysed reactions related to As, Fe and S metabolisms. This objective is addressed through an interdisciplinary approach combining geochemistry, numerical modelling, plant physiology, microbiology and omics approaches coupled with a good knowledge of the former mining sites operational management. To be sure to validate and calibrate the RTM with a robust dataset, experiments at different spatial and time scales have been conducted, notably a metric scale column experiment. This pilot experiment reproduces the different compartments of the dump: phytostabilised surface, underlying unsaturated zone, then saturated zone, with a controlled outlet discharge. A stainless-steel column was filled with 1200 kg of fine tailings from an old tin (Sn) mine. The tailings are watered at a regime close to that of the rainfall on the site, and average temperature and surface lighting (day/night) are controlled. Porewater is sampled monthly, and solids are analysed every 6 months by core sampling. The assisted phytostabilisation was started after 6 months of monitoring of the bare tailings: the surface layer was amended with limestone and compost and seeded with Festuca rubra. The tailings porewater contained, before assisted phytostabilisation, about 50 µg/L of As. This experiment demonstrates that redox reactions catalysed by microbial activities play a key role in As mobility. The following redox sequence has been indeed monitored in the water saturated level: denitrification, ferric iron reduction and reduction of AsV into AsIII, these last two reactions inducing mobilisation of As and Fe. Change in pore water chemistry is supported by the growth of an active microflora, notably AsIII-oxidising, AsV-reducing and FeIII-reducing micro-organisms, despite the low initial tailings content in microorganisms. These results were confirmed by batch experiments carried out parallel with the pilot study: slurries of tailings in water, spiked or not with low concentration of acetate, were incubated in anaerobic conditions. Results highlight that microbial activities are not limited by the amount (0.02% total organic carbon) and nature of organic matter initially present in the tailings. Experimental data allow to establish the first basis of a conceptual model of the network of stoichiometric metabolic reactions representing the redox sequence occurring in the tailings, that will support the development of a numerical model describing explicitly microbially-redox reactions as thermo-kinetically controlled reactions as well as an explicit growth of microbial population, calibrated with metagenomic and metaproteomic data. 

How to cite: Battaglia-Brunet, F., Thouin, H., Moreau, U., Milesi, V., Joulian, C., Tris, H., Charron, M., De Lary de Latour, L., Devau, N., Le Guédard, M., Pible, O., and Le Forestier, L.: Biogeochemical processes driving the fate of arsenic in phytostabilised mine tailings: elaboration of a conceptual model based on multi-scale experiments, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9451, https://doi.org/10.5194/egusphere-egu25-9451, 2025.

EGU25-11360 | ECS | Orals | ERE4.1

Removal of Arsenic in a passive treatment system for mine drainage 

Andrew Oroke, Adam Jarvis, Lucia Rodriguez Freire, and Anke Neumann

Mine drainage from abandoned mines is a major source of Arsenic (As); a ubiquitous, toxic and carcinogenic metalloid affecting over 200 million people worldwide. Recently, we observed extensive (up to 90%) co-removal of As in a vertical flow pond (VFP) passive treatment system that was designed to remove zinc from mine water drainage by precipitating ZnS following microbial sulphate reduction. However, the mechanism of As removal in the passive treatment system was unclear, even as microbial sulphate reduction is an emerging and cost-effective innovation for treating As contamination yet has received limited attention. Hence, the aim of this research was to investigate the main mechanism of As removal in the passive treatment system.

To understand the complex biogeochemical interactions of As with redox sensitive elements (Fe, S) and dissolved organic carbon (DOC), we conducted monthly field sampling over one year at the passive treatment system at the Force Crag abandoned mine site, Cumbria, UK. Aqueous sample and porewater of three depth profiles including overlying water in the VFP were collected and analysed for total element concentration, speciation (As, Fe) and DOC. Elemental composition was determined with ICP-MS. Speciation of As and Fe in aqueous phase were determined using solid phase extraction cartridges and phenanthroline method respectively, where DOC was determined with TOC Analyser.

The concentration of As (total, dissolved and colloidal) were consistently positively correlated with total, dissolved and colloidal Fe at the influent and four effluents, with concomitant decrease of both elements at the four effluents indicating potential influence of Fe on As mobility. Highest concentration of dissolved As and Fe were recorded in the porewater, which increased with depths, possibly due to vertical transportation and accumulation through the VFP, although highest level of DOC and sulphate in porewater may have caused competitive adsorption with As, resulting to weak retention of As on the binding sites. As(III) and Fe(II) were predominant in all aqueous samples, including the porewater, suggesting, to our surprise, the absence of redox transformations of As and Fe in the  VFP. Decreased As concentrations at the four effluents coincided with decreased redox potentials (anaerobic), decreased sulphate and increased DOC, indicating that organic substrates were available as electron donor and may have fuelled microbial sulphate reduction, and subsequently generating sulphide. Combined with geochemical modelling of mineral saturation indices, our results point to the precipitation of As sulphides and/or co-precipitation with Fe sulphides as the likely mechanism(s) through which As was scavenged in the treatment system. We suggest that this passive treatment system relying on microbial sulphate reduction could be further developed for treatment of As contamination in mine water effluents.

How to cite: Oroke, A., Jarvis, A., Rodriguez Freire, L., and Neumann, A.: Removal of Arsenic in a passive treatment system for mine drainage, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11360, https://doi.org/10.5194/egusphere-egu25-11360, 2025.

EGU25-12773 | Orals | ERE4.1

Preliminary paleostress study of the Kvartsevoe rare metals deposit, East Kazakhstan 

Christophe Pascal, Marina Mizernaya, Tatiana Oitseva, Eldar Salmenbayev, Dastan Tursungaliev, and Oxana Kuzmina

The Kvartsevoe rare metal deposit in East Kazakhstan was discovered in 1967 and is being currently re-evaluated after decades of inactivity. The geology of the area consists mainly of Devonian to Carboniferous metasediments, folded during the latest consolidation phase of the Altai orogen (i.e. Late Carboniferous-Permian) and intruded by series of post-kinematic Permian granites. Metals and elements of economic interest, in particular Lithium, are found in a ~300 m wide and ~700m long pegmatite body, associated with medium-earth biotite granites of phase II of the Kalba complex (i.e. 286±1 Ma). The deposit is represented by a series of pegmatite veins located in one of the projections of the Alypkelsky granite massif, the sedimentary host rocks near the deposit are hornfels of variable metamorphism up to the point of transformation into tourmaline-graphite-quartz-mica hornfels. Numerous quartz veins are found in the close vicinity of the Kvartsevoe deposit. Field observations suggest that the latter veins are genetically linked to the pegmatites. They cross-cut Permian granites and Paleozoic metasediments, show regular trends and typically extend 10s to 100s of metres. We conducted an integrated geochemical-structural study of the veins. Our preliminary results suggest vein emplacement under strike-slip stress regime with NW-SE orientation for the axis of minimum principal stress. The study seems, in addition, to confirm the genetic link between the veins and the pegmatites. Therefore, our findings suggest that the pegmatites were also emplaced under the same stress field. This latter result may be used in the future to predict the orientations of the pegmatites hosting economic metals in the subsurface.

How to cite: Pascal, C., Mizernaya, M., Oitseva, T., Salmenbayev, E., Tursungaliev, D., and Kuzmina, O.: Preliminary paleostress study of the Kvartsevoe rare metals deposit, East Kazakhstan, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12773, https://doi.org/10.5194/egusphere-egu25-12773, 2025.

EGU25-15620 | Posters on site | ERE4.1

Catchment-scale evaluation of potential particulate contaminant dispersion from post-mining sites under the effects of water erosion 

Thomas Grangeon, Rosalie Vandromme, Masson Florian, Sylvain Grangeon, Marion Ferfoglia, Stéphane Lafortune, Monique Terrier, and Olivier Cerdan

The ever-growing demand for critical resources, including metals and metalloids elements, has resulted in a dramatic increase of tailings worldwide. Tailings may contain significant concentration of potentially harmful elements like lead or arsenic. During rainfall events, runoff and associated erosion may result in contaminant dispersion to river systems, which may be particularly deleterious for ecosystems and significantly affect human health. While the massive impact of tailing dam failures has been studied in the literature, much less attention has been paid to estimating the diffuse dispersion from tailings under the effects of rainfall and runoff. Recent works however suggested that it may be a significant risk for populations, considering the significant number of tailings scattered all over the World (Macklin et al., 2023).

In the current study, more than 2000 tailings were inventoried over France. This study proposes to build a methodology to assess both the catchments structural and functional connectivity linking tailings to river channels, in a selected set of catchments located in contrasted environments (i.e. catchments located in lowland, upland and mountainous areas), in France. The proposed methodology makes use of national-scale databases, including rainfall, discharge, and suspended sediment concentration time series as well as catchments characteristics (e.g. morphology and land use). The aim of this study is to encourage discussions on the topic of catchment-scale assessment of contaminant dispersion from mining wastes under the effects of rainfall and runoff. It should ultimately help decision-makers to prioritize tailings for management plan design.

 

Macklin M.G., Thomas C.J., Mudbhatkal A., Brewer P.A., Hudson-Edwards K.A., Lewin J., Scussolini P., Eilander D., Lechner A., Owen J., Bird G., Kemp D., Mangalaa K.R. (2023). Impacts of metal mining on river systems: a global assessment. Science, 381:1345-1350.

How to cite: Grangeon, T., Vandromme, R., Florian, M., Grangeon, S., Ferfoglia, M., Lafortune, S., Terrier, M., and Cerdan, O.: Catchment-scale evaluation of potential particulate contaminant dispersion from post-mining sites under the effects of water erosion, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15620, https://doi.org/10.5194/egusphere-egu25-15620, 2025.

Smart mining integrates advanced geological, geophysical, and digital technologies—such as artificial intelligence (AI), the Internet of Things (IoT), robotics, and real-time monitoring—into traditional mining operations. This paradigm shift enhances efficiency, safety, and sustainability by enabling precise resource extraction, optimized resource management, and reduced environmental impact. As the mining industry faces challenges like resource depletion and environmental constraints, the adoption of smart mining methods becomes crucial for sustainable operations.

Central to smart mining is a high-accuracy, high-resolution, and time-lapse geological model (HHT geological model), which provides critical data for applications such as adaptive mining path planning, resource management, hazard assessment, and operational monitoring. Current geological models, while effective in some automated mining processes, lack dynamic coupling with mining equipment and disaster simulation tools, limiting their real-time applicability.

To address these limitations, we propose an integrated workflow to construct the HHT geological model: (1) Geophysical Exploration and Interpretation: Using multi-modal geophysical techniques (e.g., well logs, seismic surveys, transient electromagnetics), we invert geological properties (e.g., seismic impedance, wave speed, resistivity) and interpret structural features such as horizons, faults, voids, rock facies, and mineral boundaries. (2) Model Generation: Employing Triangulated Irregular Network (TIN) methods to create a detailed 3D geological framework. (3) Dynamic Updates via Continuous Monitoring: Utilizing data from seismic while mining (SWM), 4D seismic, and joint microseismic-electromagnetic monitoring to update the geological model as mining progresses.

The Key Innovations of our proposed workflow have three aspects: (1) we integrate geological, petrological, seismic, and electromagnetic data, combined with mining-induced seismic events, machinery running parameters, and video/image recognition technologies to enable high-resolution imaging and detection of coal seam thickness, fault zones, goaf areas, and subsidence columns, providing a comprehensive understanding of geological structures. (2) We apply Seismic While Mining (SWM) technology, which acquires continuous seismic data during mining operations, processed through reverse-time migration, cross-correlation, denoising, and source wavelet extraction, to dynamically image geological changes. A six-component seismometer further enhances constraints via virtual sonic well logging. (3) We apply the Real-time TIN regeneration method which incorporates the discrepancies between SWM-derived images and the prior model, ensuring accurate updates during mining.

We tested the platform in an underground coal mine near Erdos, Inner Mongolia, China, the SWM method successfully identified faults along a tunnel, later confirmed by mining reports. These results demonstrate the effectiveness of the integrated HHT geological model in revealing hidden geological features.

In conclusion, the HHT geological modeling is fundamental for realizing true smart mining. Merging multi-source geophysical data establishes a reliable seismic baseline, while the SWM system provides critical real-time monitoring of roof deformation, stress distribution, water infiltration, and rock bursts. The integration of these methods is essential to achieving a "transparent geological model" and advancing towards sustainable and intelligent mining practices.

How to cite: Zhou, T.: Towards Smart Mining: An Integrated Process for High-Accuracy, High-Resolution, and Time-Lapse Geological Modeling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15713, https://doi.org/10.5194/egusphere-egu25-15713, 2025.

EGU25-15851 | ECS | Posters on site | ERE4.1

Numerical Simulation of the Effect of Vegetation on Infiltration in Soil Covers of Potash Tailings Piles 

Felipe Edgardo Silva Monsalves and Thomas Graf

Potash tailings piles from the mining of potassium salts present considerable environmental challenges concerning surface and groundwater. Uncovered piles are primarily composed of saline residues such as sodium chloride, magnesium sulfate and magnesium chloride. To mitigate the interaction between saline residues and rainwater, some piles have been covered by different soil types in some regions of the world, including Germany, to act as a physical barrier to prevent water-salt contact. In this way, the amount of infiltrated water is reduced, thereby reducing the amount of salts that can be leached and transported to the underlying water bodies. The extent to which the soil cover prevents the contact of infiltrated rainwater will depend on the hydraulic parameters of each soil type, how many soil layers make up the overall soil cover, how the soil layers are distributed, and on the hydrological situation of each region. While climatic factors such as precipitation are fundamental controlling factors, the type and distribution of vegetation play a crucial role in the efficiency of the pile cover. The objective of this research is therefore to quantify the effect of vegetation on infiltration and evapotranspiration in a vegetated soil cover over a hypothetical potash tailings pile by numerical simulation. For this purpose, different types of vegetation are analyzed, represented by their hydrological parameters leaf area index, depth and root density. The seasonal variations of the vegetation represented by temporally changing parameter values are also taken into consideration. Different depths of the cultivation layer for vegetation, the stabilization layer, the drainage layer and the sealing layer are regarded. The numerical simulation is carried out with the Advanced Terrestrial Simulator (ATS), a software which allows surface-subsurface coupling through continuity conditions of pressure in both zones. The software solves the diffusion wave equation for surface flow and Richard’s equation for the subsurface flow. Additionally, ATS implements the Priestley-Taylor model for potential evapotranspiration. Together with vegetation parameters, this enables the calculation of actual evapotranspiration and, subsequently, the water balance of the soil cover. Results from 2D simulations demonstrate the ability of the model to represent the relevant coupled processes outlined above. The simulated infiltration patterns provide valuable insights for optimizing cover design and vegetation selection, contributing to the development of more effective solutions for groundwater protection in potash tailings piles areas.

How to cite: Silva Monsalves, F. E. and Graf, T.: Numerical Simulation of the Effect of Vegetation on Infiltration in Soil Covers of Potash Tailings Piles, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15851, https://doi.org/10.5194/egusphere-egu25-15851, 2025.

EGU25-16097 | ECS | Orals | ERE4.1

A Cutting-Edge Framework for Sustainable Phosphate Waste Characterization Using Hyperspectral Imaging and Machine Learning 

Abdelhak El Mansour, Ahmed Laamrani, Abdellatif Elghali, Rachid Hakkou, and Mostafa Benzaazoua

Abstract

Management of phosphate mine waste rock piles (PWRPs) is a critical challenge in the mining industry, particularly in regions like Morocco, which holds the world’s largest phosphate reserves. To this end, there is a need for an approach that focuses on real-time monitoring of waste rock heterogeneity, enabling more efficient resource recovery and environmental management. This study proposes a novel, multi-scale approach that integrates hyperspectral imaging, field spectroscopy, and explainable machine learning (XML) to characterize and map the mineralogical diversity of PWRPs at the Benguerir mine.  A total of 103 samples were collected from waste rock piles across an area of approximately 60 km², representing the full spectrum of mineralogical variability. Handheld X-ray fluorescence (XRF) analysis was conducted on the all the samples and revealed the dominance of SiO₂ (29.51 wt% ± 12.42), CaO (30.16 wt% ± 10.17), and P₂O₅ (7.23 wt% ± 4.21). These XRF analyses indicated the presence of silicate, carbonate, and phosphate-bearing materials. These findings were complemented by both PRISMA hyperspectral imaging, which captured spectral data across the visible to shortwave infrared (VSWIR) range. precise calibration and validation of the remote sensing outputs were conducted using field spectroscopy using the ASD FieldSpec 4 spectroradiometer.

To address the complexity of the spectral data, we developed an explainable machine learning framework based on SHapley Additive exPlanations (SHAP) and Convolutional Neural Networks (CNN). This framework not only improved classification accuracy (achieving 0.92 overall accuracy) but also provided interpretable insights into the spectral features driving mineral identification. Our results showed that the used model successfully differentiated four main waste rock categories: carbonate-rich, phosphate-rich, clay-dominated, and siliceous materials. The resulting maps offer a practical tool for real-time waste management and resource recovery. For instance, carbonate-rich materials, characterized by high CaO content, can be identified or used for construction applications, while phosphate-rich zones, with elevated P₂O₅ levels, can be flagged for potential recovery and further processing. This targeted approach ensures that waste materials are repurposed efficiently, aligning with circular economy principles. The study highlights the potential for automated, spectroscopy-based monitoring systems to support sustainable mining practices. Overall, this study demonstrates the power of combining cutting-edge remote sensing technologies with explainable machine learning to address the challenges of phosphate waste rock characterization. The methodology provides a scalable, cost-effective solution for mining operations worldwide, with significant implications for environmental sustainability, resource efficiency, and circular economy initiatives.

Keywords: Phosphate mine waste, Hyperspectral imaging, Field spectroscopy, Explainable machine learning (XML), Sustainable mining.

How to cite: El Mansour, A., Laamrani, A., Elghali, A., Hakkou, R., and Benzaazoua, M.: A Cutting-Edge Framework for Sustainable Phosphate Waste Characterization Using Hyperspectral Imaging and Machine Learning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16097, https://doi.org/10.5194/egusphere-egu25-16097, 2025.

EGU25-16370 | Orals | ERE4.1

Advancing Multivariate Simulations using Non-Euclidean Metrics 

Andrew Pavlides, Maria Despoina Koltsidopoulou, Maria Chrysanthi, and Emmanouil Varouchakis

Multivariate data analysis in natural resources exploration can be beneficial for each variable investigated as the correlation between the variables increases the prediction accuracy and reduces the error variance. Geostatistical modeling of mineral deposits often encounters challenges in accurately representing spatial dependencies, particularly in complex geological formations and irregular sampling grids. While traditional Euclidean distances are commonly used, they may not adequately capture spatial relationships in such scenarios. Non-Euclidean distances, such as Manhattan and Chebyshev metrics, as well as geodesic distance (like a sphere manifold), offer alternative solutions that may better accommodate spatial fields with complex sampling grids. Such distances however may result in non-positive definite (thus not invertible) covariance matrices. This is further complicated when dealing with multivariate random fields as the resulting covariance-cross-covariance matrix may not be positive-definitive even in the Euclidean distance.

This study builds on prior research to evaluate spatial dependencies for Aluminum (Al) and Zinc (Zn) concentrations in geochemical datasets under both Euclidean and non-Euclidean distance metrics. The data values have undergone Gaussian Anamorphosis with the previously introduced CDKC method. The recently introduced Harmonic Covariance Estimation (HCE) model is applied to generate covariance structures for co-kriging predictions, as well as multivariate simulations. Such simulations can assist in exploring the uncertainty of estimation (for example the 90% confidence interval) after the back-transform. The ability of HCE to maintain positive-definite cross-covariance matrices is a critical focus, particularly in multivariate simulations.

In addition, this work investigates a separate dataset from a mine in Ireland, which includes Lead (Pb) and Zinc (Zn) concentrations. Here, the anisotropic form of the HCE model introduced and then applied in Euclidean space to account for directional dependencies. The performance of anisotropic HCE is then compared to kriging predictions using non-anisotropic HCE with non-Euclidean distances (Chebyshev, Manhattan, Spherical Manifold). This analysis aims to determine whether correcting for anisotropy or adopting non-Euclidean metrics yields better performance in this particular dataset, although more studies are required to reach a conclusion on the matter.

The investigation results indicate that the HCE model results in invertible, positive-definite matrices that can be used for simulations and predictions with non-Euclidean distances, offering insights into optimizing spatial modeling for irregular datasets and complex deposit structures.

 

The research project is implemented in the framework of H.F.R.I call “Basic research Financing (Horizontal support of all Sciences)” under the National Recovery and Resilience Plan “Greece 2.0” funded by the European Union – NextGenerationEU (H.F.R.I. Project Number: 16537)

How to cite: Pavlides, A., Koltsidopoulou, M. D., Chrysanthi, M., and Varouchakis, E.: Advancing Multivariate Simulations using Non-Euclidean Metrics, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16370, https://doi.org/10.5194/egusphere-egu25-16370, 2025.

EGU25-17455 | Orals | ERE4.1

Automated mineral sensing for robotic miners: the ROBOMINERS perception payload 

Christian Burlet and Giorgia Stasi

ROBOMINERS (Bio-Inspired, Modular and Reconfigurable Robot Miners, Grant Agreement No. 820971, http://www.robominers.eu) was a European project funded by the European Commission's Horizon 2020 Framework Programme. The project aimed to test and demonstrate new mining and sensing technologies on a small robot-miner prototype (~1-2T) designed to target unconventional and uneconomical mineral deposits (technology readiness level 4 to 5).

As part of the ROBOMINERS sensors payload development, a set of mineralogical and geophysical sensors were designed to provide the necessary data to achieve “selective mining”, the ability to reduce mining waste production and to increase productivity of small mining machines. The robot should have the ability to react and adapt in real time to geological changes as it progresses through a mineralized body. The perception payload technologies demonstrated in the project are based on reflectance/fluorescence spectroscopy, laser-induced breakdown spectroscopy and Electrical Resistivity Tomography.

The field trials of the sensors have been carried out in the entrance of abandoned mine (baryte and lead mine, Ave-et-Auffe, Belgium), as well as in an open pit mine (bituminous shales mine in Kunda, Estonia) and in an underground lead mine (Mezica, Slovenia). These tests allowed to demonstrate the effectiveness of these sensors to provide realtime to sub-realtime mineralogical and geophysical data to a robotic drilling platform, paving the way for more autonomy in robotized mining machines.

How to cite: Burlet, C. and Stasi, G.: Automated mineral sensing for robotic miners: the ROBOMINERS perception payload, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17455, https://doi.org/10.5194/egusphere-egu25-17455, 2025.

EGU25-17917 | ECS | Posters on site | ERE4.1

Stabilizing hazardous mine waste in alkali-activated geopolymers for pollution mitigation at abandoned mining sites 

Jihene Nouairi, Slavka Andrejkovičová, Omaima Karoui, Tiago Pinho, Rafael Rebelo, Gil Gonçalves, Angelo Camerlenghi, Mounir Ghribi, and Fernando Rocha

The use of alkali-activated materials presents a sustainable approach to replacing conventional construction resources while promoting waste valorization, in line with the goals of the blue economy for environmentally responsible development. This study explores the innovative use of mine waste (MW) from an abandoned lead-zinc (Pb-Zn) mining site in Northern Tunisia as a cost-effective, high-adsorption additive in the production of metakaolin-based geopolymers. Metakaolin (sourced from Vicente Pereira, Ovar, Portugal) was partially substituted with MW in varying proportions (0%, 5%, 10%, 20%, and 30%). The geopolymer formulations maintained constant molar ratios of SiO₂/Al₂O₃ and Na₂O/Al₂O₃ at 1 to minimize the use of sodium silicate and sodium hydroxide, leading to the development of environmentally friendly geopolymers with a reduced carbon footprint.

The study assessed how the incorporation of MW influences the geopolymers' microstructure, mechanical strength, and ability to adsorb methylene blue dye. Chemical analysis of MW revealed elevated concentrations of hazardous elements, up to 2.23 wt.% Pb and 8.2 wt.% Zn, highlighting the importance of stabilizing these elements to prevent environmental contamination. Scanning Electron Microscopy (SEM) indicated varying degrees of geopolymerization across different formulations, predominantly featuring amorphous phases. After 28 days of curing, samples with 5 wt.% and 10 wt.% MW exhibited the highest compressive strengths of 25 MPa and 30 MPa, respectively.

The adsorption capacity of the developed geopolymers was evaluated using Methylene Blue (MB) dye, with experiments focusing on the effects of adsorbent dosage and contact time. Adsorption kinetics closely followed the pseudo-second-order model, while the Langmuir isotherm model best described the adsorption behavior. Notably, samples with 30 wt.% and 0 wt.% MW achieved the highest adsorption capacities, demonstrating the beneficial role of MW in enhancing the properties of alkali-activated metakaolin geopolymers and its potential to partially substitute metakaolin.

How to cite: Nouairi, J., Andrejkovičová, S., Karoui, O., Pinho, T., Rebelo, R., Gonçalves, G., Camerlenghi, A., Ghribi, M., and Rocha, F.: Stabilizing hazardous mine waste in alkali-activated geopolymers for pollution mitigation at abandoned mining sites, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17917, https://doi.org/10.5194/egusphere-egu25-17917, 2025.

EGU25-18583 | ECS | Posters on site | ERE4.1

Geodatabase of Sinkholes in the the Post-Mining Area of the Brown Coal Mine “Babina” (W Poland) 

Natalia Walerysiak and Jan Blachowski

Post-mining sites are prone to complex processes related to the ceased mining and disturbance of the rock mass around the excavations. Therefore, such sites require continuous monitoring to minimize threats associated with, e.g. occurrence of often unexpected discontinuous deformations such as sinkholes. This study focuses on the development and analysis of a database of sinkholes in the former “Babina” brown coal mine in Western Poland. The mine site is located in the SW part of the complex glaciotectonic area of the “Muskau Arch”. It was subjected to long-term open-pit and shallow underground mining. The primary objective of the study is to create a comprehensive database of sinkholes, based on analysis of differential digital elevation model and derivatives of digital elevation model such as slope and hillshade maps. The structure of the database includes dependent variables such as geographical location and dimensions of sinkholes, as well as parameters representing potential causative factors including: geological, mining, geophysical and topographical characteristics (exploratory variables). It will be used to analyse and model the relationship of sinkhole occurrence with potential causative factors of their occurrence in the project no. 2021/43/B/ST10/02157.

The geodatabase was developed using ArcGIS software from ESRI, encompassing information on more than 230 identified sinkholes. Each sinkhole in the database is comprehensively described by a range of attributes. The exploratory variables include total depth of mining, distance to the first underground level, distance to shafts and adits, location of brown coal outcrops locally named gizers, proximity to coal seams (geological mining factors). Among the topographical factors the following attributes have been stored: slope of the terrain, distances to former open pits, anthropogenic lakes and waste heaps, land cover types. The geophysical data include results of gravimetric observations (anomalies in the gravitational field). Whereas, the hydrogeological data include results of underground water modelling.

The construction of the database was done by using advanced spatial data processing tools such as Map Algebra Statistics and Surface Functions, as well as extract value to feature tools. These functions were used to calculate and to extract raster values associated with location of sinkholes in addition distance tools where used to determine parameters derived from vector data that include for example database of underground working.

The dataset was subjected to a comprehensive statistical analysis, which included developing descriptive statistics encompassing histograms of the values of dependent variables (sinkhole parameters) and independent variables (factors potentially influencing the formation of deformations). An exploratory data analysis was also conducted to determine correlations between variables.

The results of the study have allowed analysing weighted spatial distribution of sinkholes in the post-ming area. The weights included parameters of sinkholes. Further research is aimed at developing predictive models with a machine learning approach. The models will be used to identify areas prone to future sinkhole formation.

The results of the study confirm the complexity of post-mining impacts and the necessity for further detailed analysis of the changes taking place in the study area.

The research has been financed from the OPUS National Science Centre projects grants no. 2019/33/B/ST10/02975 and no. 2021/43/B/ST10/02157.

How to cite: Walerysiak, N. and Blachowski, J.: Geodatabase of Sinkholes in the the Post-Mining Area of the Brown Coal Mine “Babina” (W Poland), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18583, https://doi.org/10.5194/egusphere-egu25-18583, 2025.

EGU25-18653 | ECS | Orals | ERE4.1

UTLD: An Underground Thermal and LiDAR Dataset for Depth Estimation 

Zhihua Xu, Jiaxuan Lin, Qingxia Ye, and Zengyi Guo
  • Introduction

Depth estimation is a crucial task in photogrammetry and computer vision. The underground scenes, characterized by low-light conditions, high dusty, and narrow structures, pose challenges in depth estimation using existing visual-based datasets. We provide an Underground Thermal image and Lidar Dataset (UTLD) for depth estimation over underground scenes. It contains stereo thermal images and the corresponding point clouds achieved by stereo laser scanners over three different underground mines. We tested some monocular depth estimation methods on the UTLD dataset to highlight the challenges and opportunities. Figures 1-2 show the acquisition scenes and platforms, respectively.

Figure. 1. UTLD dataset real collection environment

Figure. 2. Data Collection Platform

  • Method Testing

We selected four existing monocular depth estimation methods, each implemented using their official source codes. Figure 3 compares the depth maps of different mathods on the dataset. The methods predict large objects well but struggle with distant targets and fine-grained details. Nevertheless, they capture the geometric structures. Besides, we presents the evaluation metrics for these methods on the UTLD dataset, where the PixelFormer method achieves the best performances (not included in the text).

   

Figure. 3. Depth maps of different methods on the UTLD dataset.

  • Conclusion & Prospects

This study introduces the UTLD dataset and validates the feasibility of monocular depth estimation methods in underground mines. In future work, we will improve the image quality under high dust underground scenes. Besides, semantic segmentation will be involved to promote the practical adoption of vision systems in smart applications of underground mines.

How to cite: Xu, Z., Lin, J., Ye, Q., and Guo, Z.: UTLD: An Underground Thermal and LiDAR Dataset for Depth Estimation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18653, https://doi.org/10.5194/egusphere-egu25-18653, 2025.

EGU25-18711 * | Orals | ERE4.1 | Highlight

Invisible Mining: A Novel Approach to Addressing EU Critical Raw Materials Challenges 

Marko Komac, Vitor Correia, and Eberhard Falck

Overview/Background

The European Union faces significant challenges in securing critical raw materials (CRM) while balancing environmental protection, public acceptance, and technological innovation. This research examines how innovative "invisible mining" approaches, enabled by advances in robotics and miniaturisation, could help resolve conflicts between mineral extraction needs and environmental preservation goals, particularly in the context of the EU's Critical Raw Materials Act (CRMA). This paper addresses the growing tension between increased raw material demand for green technologies and the EU's stringent environmental protection mandates.

 

Methods

We analysed the intersection of technological innovation, policy frameworks, and social acceptance through a comprehensive review of EU-funded research projects in mining automation and robotics. We evaluated six major research initiatives from 2011-2026, examining their technological developments and potential applications. The analysis incorporates findings from case studies of mining operations in environmentally sensitive areas and assesses the viability of emerging business models in the mining sector. Special attention was given to projects developing autonomous robotic systems for underground operations and advanced sensing technologies for precise mineral extraction.

 

Results

The research identifies four key transformative elements for successful implementation of invisible mining: (1) technological advances in robotics and miniaturisation enabling precise, low-impact extraction through smaller diameter galleries and reduced waste rock production; (2) comprehensive and integrated resource recovery principles maximising resource efficiency while minimising environmental disturbance; (3) materials-as-a-service business models creating circular resource loops and transforming mining companies from mere extractors to long-term material stewards; and (4) development of new workforce competencies in advanced cognitive domains such as robotics, data science, and environmental management. The analysis reveals that more than 80% of CRM deposits in Europe are located near or within environmentally protected areas, highlighting the urgent need for innovative extraction approaches. Additionally, the study demonstrates how autonomous mining systems can operate in narrow drifts without human presence, eliminating the need for extensive ventilation and drainage systems.

 

Conclusions

The findings demonstrate that invisible mining, characterised by minimal surface disturbance and environmental impact, represents a viable solution to the EU's raw materials challenges. This approach, combined with new business models and advanced technologies, could significantly increase public acceptance of mining activities while meeting the EU's resource needs. Success requires a fundamental transformation of the mining sector, encompassing technological innovation, business model evolution, and workforce development. The research suggests that invisible mining could enable the coexistence of resource extraction and environmental protection, particularly in sensitive areas, while supporting the EU's transition to a green economy. The study emphasises that this transformation demands sustained investment in robotics research, development of circular economy practices, and reimagining of traditional mining business models to create a more sustainable and socially acceptable mining industry.

How to cite: Komac, M., Correia, V., and Falck, E.: Invisible Mining: A Novel Approach to Addressing EU Critical Raw Materials Challenges, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18711, https://doi.org/10.5194/egusphere-egu25-18711, 2025.

EGU25-19608 | ECS | Posters on site | ERE4.1

The PERSEPHONE project: Autonomous Exploration and Extraction of Deep Mineral Deposits 

Akash Patel, Anton Koval, Sumeet Gajanan Satpute, George Nikolakopoulos, Christian Burlet, and Giorgia Stasi

PERSEPHONE is a Horizon Europe project (Grant Agreement No.101138451) dedicated to autonomous exploration and extraction of deep mineral deposits. The project has been created in support to the increasing demand for raw materials, which compel European mining companies to extract ore at greater depths. In this framework, current mining operations and traditional technologies face significant challenges in maintaining profitability while aligning with the European Green Deal's environmental objectives and ensuring worker safety. 

To address these challenges and enable sustainable development, PERSEPHONE focuses on developing innovative technologies for resource-efficient extraction and near-mine exploration of critical raw materials. PERSEPHONE’s vision includes reducing the scale of mining equipment to optimize operations in challenging environments, integrating autonomous systems for risk-aware navigation, and digitalization of the extraction process. A key innovation is the creation of digital twins, supported by the validation of key enabling technologies at Technology Readiness Level 5 (TRL 5). Additionally, the project introduces groundbreaking approaches to online near-mine exploration, core analysis, and advanced data analytics for mine expansion and decision support. 

In the first half of the project, several of its key technologies have been tested in the laboratory and controlled underground environments at mine sites. More specifically, the initial tests of autonomy stack for high accuracy navigation have been carried out. Additionally, a multispectral camera has been integrated with a developed autonomy package that combines 3D LiDAR and RGB-D camera. This payload has been mounted on the Unitree robotic platform for the initial combined data collection. 

Ultimately, PERSEPHONE aims to digitalize and automate the mining value chain, advancing towards sustainable, efficient, and safe exploration and extraction practices. The project contributes significantly to achieving the EU’s critical raw material goals while supporting the transition to a greener economy. 

How to cite: Patel, A., Koval, A., Satpute, S. G., Nikolakopoulos, G., Burlet, C., and Stasi, G.: The PERSEPHONE project: Autonomous Exploration and Extraction of Deep Mineral Deposits, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19608, https://doi.org/10.5194/egusphere-egu25-19608, 2025.

EGU25-19825 | ECS | Posters on site | ERE4.1

Assessing SWIR and MWIR Hyperspectral Imaging for Rapid Estimation of P2O5 Distribution in Sedimentary Phosphate Drill Cores 

Mohamed Mazigh, Otmane Raji, and Mostafa Benzaazoua

Sedimentary phosphate rocks are crucial for global food security, contributing to over 90% of the fertilizer industry's needs. However, their exploration and mining face significant challenges due to substantial horizontal and vertical variations in phosphorus concentrations within the strata. Traditional characterization methods are time-consuming and costly, requiring complex sample preparation, which often limits the spatial resolution of measurements across the ore body. On the other hand, infrared hyperspectral core scanning has emerged as a proven technique for rapid characterization of mineral assemblages along drill cores, which by leveraging advanced machine learning algorithms, offers a powerful tool for predicting geochemical variations. In this context, our study aims to assess the ability of hyperspectral infrared imagery to rapidly quantify the distribution of P₂O₅ in phosphate drill cores using a non-destructive methodology. For this, a ~65-meter drill core from the phosphatic series of Ben Guerir (Morocco) was analyzed. P₂O₅ measurements were acquired using a Thermo Fisher XL5 portable XRF (pXRF), and hyperspectral images were collected using a SPECIM SisuROCK core-scanner with SWIR (1000–2500 nm) and MWIR (2700–5200 nm) cameras. To predict P₂O₅ concentrations from infrared spectra recorded in hyperspectral imagery, we explored a direct method, using high-performing machine learning algorithms trained on a ~5-meter drill core dataset. When applied to the whole drill core dataset, the machine learning algorithms—Random Forest Regressor, KernelRidge Regressor, Gradient Boosting, Support Vector Regressor, and K-Nearest Neighbors— reported good predictive performance with strong correlations of 78%, 78.2%, 67.1%, 74.9%, and 68.7% in the SWIR region and 81.2%, 83%, 80.2%, 83.24%, and 82% in the MWIR region, respectively. Direct estimation of P₂O₅ using the Support Victor Regression model on MWIR imagery thus represents a more effective approach, offering significant potential for P₂O₅ chemical mapping and improved phosphorus resource estimation with a low mean absolute error of 3.29. Further improvements could be achieved by employing a larger training dataset and deep learning algorithms.

How to cite: Mazigh, M., Raji, O., and Benzaazoua, M.: Assessing SWIR and MWIR Hyperspectral Imaging for Rapid Estimation of P2O5 Distribution in Sedimentary Phosphate Drill Cores, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19825, https://doi.org/10.5194/egusphere-egu25-19825, 2025.

EGU25-19998 | ECS | Orals | ERE4.1

Assesment for Water Flow and Solute Transport in Tailings Piles: a numerical modeling to design an artificial tracer test 

Wilfredo Puelles-Ramírez, Anne Jost, Pierre L'Hermite, Michael Descostes, Benoît Reilé, and Valérie Plagnes

The former uranium mine, Le Cellier, located in South of France, offers an opportunity to investigate the unsaturated flow and solute transport through a tailings pile resulting from heap leaching under real-world conditions (Ouedraogo et al., 2022; L’Hermite et al., 2024). Numerical simulations of one of the tailings pile were conducted to model the dynamics of the water flow. In order to tackle quality issues and to validate the hydrogeological model, we plan to make an artificial tracing test experiment. We developed a solute transport model for this pile to help the design of this experiment that will be carried out in the next future.

Conceptual one-dimensional (1D) systems representing the pile were simulated using the HYDRUS code for flow and conservative transport. The first results show that the model generates breakthrough curves exhibiting the same dynamics, irrespective of the top concentration of the injected dissolved solute. High values of hydraulic conductivity and longitudinal dispersivity accelerates solute transport, resulting in higher concentration peaks. Dual-porosity models yield significantly shorter residence times compared to single-porosity models, particularly during dry periods. The impact of climatic conditions before and during the tracer injection as well as the injection method have been also evaluated with this model.   

These findings suggest that artificial tracer experiments in the studied pile should be conducted under wet conditions and give useful information for the field implementation of the test. This simulation approach provides valuable insights for designing effective and realistic tracer test experiments. Our study shows that this type of field and modeling approach of tracer testing can help in mine water management strategies.

How to cite: Puelles-Ramírez, W., Jost, A., L'Hermite, P., Descostes, M., Reilé, B., and Plagnes, V.: Assesment for Water Flow and Solute Transport in Tailings Piles: a numerical modeling to design an artificial tracer test, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19998, https://doi.org/10.5194/egusphere-egu25-19998, 2025.

EGU25-21220 | Orals | ERE4.1

Assessing the Critical Raw Materials potential in Europe to support the energy transition. 

Guillaume Bertrand, Capucine Albert, and Alex Vella

The energy transition imposes to Europe the crucial challenge of securing a sustainable supply of critical raw materials (CRMs). The European Union's Critical Raw Materials Act represents a strategic response to this challenge, aiming to strengthen Europe's supply chain resilience and reduce dependence on foreign imports for materials essential to green technologies. Assessing Europe's domestic potential for CRMs is fundamental to achieving the Act's objectives of securing 10% of the EU's annual consumption through domestic extraction by 2030. This evaluation becomes particularly vital as demand for these materials is projected to surge with the widespread adoption of renewable energy technologies, electric vehicles, and energy storage systems.

In this context, European geological survey organizations (GSOs) play a key role, at national to EU levels. The EU-funded GSEU – Geological Service for Europe project, coordinated by EuroGeoSurveys, an international organization that brings together Europeans GSOs, aims at providing harmonized pan-European geoscientific data and expertise to support policy and decision making. The Raw Materials team, coordinated by BRGM, the French geological survey organization, has compiled a harmonized dataset of CRM deposits in Europe, controlled and updated by all national data providers, based on the 2023 CRM list of the European Commission. This dataset allows to assess and map the geological potential for CRM in Europe, globaly, per country and per commodity.

In addition to a harmonized and updated knowledge on the geological potential in Europe, mineral prospectivity mapping (MPM) plays a pivotal role by identifying areas with high potential for the discovery of new CRM deposits. Based on the harmonized dataset of CRM deposits in Europe produced by the GSEU Raw Materials team, the 1 to 1.5M lithostratigraphic and structural maps of Europe and a new data driven MPM method combining the DBA (Disc Based Association) data aggregation approach and Random Forest regression, we have produced pan-European prospectivity maps for a selection of CRM (Co, Cu, Li, Ni, Mg, Mn, Nb, Ni, Sb, Ta, V, W). These maps provide crucial information to both industry stakeholders and policymakers. They reduce exploration risks and costs by highlighting promising areas for detailed investigation, and they enable informed decisions about land use, environmental protection and resource management strategies.

In this presentation, we briefly describe the CRM deposits dataset compiled by the GSEU Raw Materials team, the maps and potential assessments for CRM in Europe, and the pan-European mineral prospectivity maps for selected critical commodities. We also briefly present the methodologies that were used to develop these products and discuss future developments of this work.

How to cite: Bertrand, G., Albert, C., and Vella, A.: Assessing the Critical Raw Materials potential in Europe to support the energy transition., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21220, https://doi.org/10.5194/egusphere-egu25-21220, 2025.

EGU25-21303 | Orals | ERE4.1

A continent-scale data-driven approach to map Critical Raw Materials potential in Europe 

Alex Vella, Guillaume Bertrand, Charles Gumiaux, and Capucine Albert

The energy transition presents a crucial challenge to Europe, with the necessity of securing a sustainable supply of Critical Raw Materials (CRM) as specified in the European Union's Critical Raw Materials Act. Reaching the goal set by the Act of securing 10% of the EU's annual consumption through domestic extraction by 2030 requires the assessment of Europe’s domestic potential for CRMs. The collection of available data regarding the known CRMs potential throughout Europe is needed to perform this assessment. This data collection allows to perform mineral potential mapping to highlight areas with potential for the discovery of new CRM deposits.

The EU-funded GSEU – Geological Service for Europe project, coordinated by EuroGeoSurveys, an international organization that brings together Europeans geological survey organizations, aims at providing harmonized pan-European geoscientific data and expertise to support policy and decision making. As part of this project, mineral prospectivity mapping methods are applied to outline areas with the highest likelihood to host potential mineralization. They allowed the production of pan-European prospectivity maps for a selection of CRM (Co, Cu, Li, Ni, Mg, Mn, Nb, Ni, Sb, Ta, V, W). Favorability maps highlight promising areas for mineral exploration, improving exploration benefit/costs ratio, reducing its environmental footprint and enabling informed decisions about land use, environmental protection, and resource management strategies. They provide crucial information to both industry stakeholders and policymakers.

These maps are produced using the “Disc-Based Association” (DBA) method in combination with a Random Forest supervised classification. This predominantly data-driven approach leverages spatial analysis and machine learning techniques to delineate prospective zones for mineral exploration, specifically targeting CRMs. The DBA method analyses neighboring associations of cartographic features over the studied area, producing a unique matrix presenting the multivariate features identified around each sample point. The Random Forest classification allows scoring of each sample points through a binary classification. The first class consist of sample points in the vicinity of known mineralization, accessed through the harmonized dataset of CRM deposits provided by the GSEU Raw Materials team, while the second class are all the other sample points. The classification process results in each point being given a score, displaying the favorability of an area for mineral exploration. The result of this classification allows the definition of favorable areas for mineral exploration throughout Europe.

In this presentation, we describe the methodology used to produce the favorability maps for CRMs in Europe using the data compiled by the GSEU Raw Materials team. We present some of the resulting favorability maps and discuss future developments and application of this methodology.

How to cite: Vella, A., Bertrand, G., Gumiaux, C., and Albert, C.: A continent-scale data-driven approach to map Critical Raw Materials potential in Europe, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21303, https://doi.org/10.5194/egusphere-egu25-21303, 2025.

EGU25-2356 | ECS | Posters on site | ERE6.2

Maximising Benefits of Sustainable Development Target Interactions: An Integrated Priority Analytical Model Applied to China 

Yuanhui Wang, Rotem Zelingher, Nikita Strelkovskii, Changqing Song, and Peichao Gao

National governance plays a pivotal role in achieving the 2030 Sustainable Development Goals (SDGs) under limited resources. Therefore, it is necessary to prioritize SDGs and their underlying targets to support informed decision-making. Among the scientific approaches, integrated priority analytical models have led to the consideration of interwoven interactions among targets and the involvement of both traditional analytical and interaction-related criteria. However, existing models have limitations in maximizing the benefits of interactions, as they tend to overlook negative and high-order interactions. To address this issue, this study proposes a new model that integrates impacts of direction-specific high-order interactions and temporal trends in a tri-dimensional framework to assign target-specific “temporal priorities” and “resource priorities” at the national scale. We applied this model to the priority analysis of SDG targets in China to demonstrate its usefulness in leveraging the benefits of interactions within a complex sustainability framework. Our analysis shows that, for temporal priorities, 10.7% of targets require urgent action to promote progress or address trade-offs, and 23.8% demand low levels of urgency. The urgent targets focus on energy efficiency, augmented funding for forest management, and biodiversity preservation. Concerning resource priorities, 27.4% of targets necessitate elevated resource allocation, clustering primarily within Goals 12, 15, and 16. Accordingly, we recommend policy actions to enhance funding for biodiversity preservation and forest management and to foster energy efficiency measures. Additionally, allocating extra resources to the responsible consumption goal is imperative due to pronounced trade-off effects.

How to cite: Wang, Y., Zelingher, R., Strelkovskii, N., Song, C., and Gao, P.: Maximising Benefits of Sustainable Development Target Interactions: An Integrated Priority Analytical Model Applied to China, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2356, https://doi.org/10.5194/egusphere-egu25-2356, 2025.

EGU25-2451 | ECS | Posters on site | ERE6.2

Developing a Life Cycle Assessment Framework with Nature-based Solutions for Carbon Footprint Management in Irrigation Infrastructure 

Chung Yu Yang Hung, Yi Ju Chen, Wei Chun Chuang, and Ching Pin Tung

Irrigation infrastructure, critical for agricultural water management, contributes significantly to greenhouse gas (GHG) emissions during its operational phase due to energy and resource consumption for gate operations, water pumping, and maintenance activities. In Taiwan, the construction of new irrigation canals has largely plateaued, with current projects predominantly focusing on repair, replacement, and upgrades. This study seeks to address the carbon footprint of these engineering activities by developing a tailored Life Cycle Assessment (LCA) framework that evaluates emissions hotspots specific to irrigation infrastructure and explores Nature-based Solutions (NbS) as mitigation strategies.

The LCA framework focuses on the maintenance and operational stages (B1-B5) of irrigation systems while incorporating end-of-life considerations (C1-C4) where necessary. For instance, it assesses energy consumption during post-repair operations and simulates scenarios involving energy savings or material reuse. NbS interventions, such as vegetative soil stabilization, eco-friendly repair techniques, and energy-efficient water management systems, are analyzed for their feasibility and alignment with the eight NbS criteria and twenty-eight associated indicators. The framework is designed to quantify the potential of these interventions to reduce lifecycle emissions and enhance ecosystem resilience.

Aligned with the Global Ecosystem Research Infrastructures Initiative, this study incorporates harmonized methodologies and collaborative practices to evaluate carbon emissions and explore effective mitigation strategies. By addressing key environmental challenges through structured frameworks, the research highlights the potential for interoperability and scalability, offering insights into how localized practices can inform global efforts in sustainable water resource management and climate resilience.

Preliminary findings highlight the potential of NbS to address key emission sources. For example, vegetative solutions applied to embankments reduce soil erosion while simultaneously sequestering carbon, and energy-efficient upgrades to water pumping systems significantly lower operational emissions. These results underscore the value of integrating LCA with NbS to provide actionable pathways for mitigating environmental impacts while ensuring infrastructure functionality.

By focusing on a localized case study of Taiwan’s irrigation infrastructure, this research demonstrates how regional practices can contribute to global environmental research infrastructures, fostering collaboration and advancing efforts to address shared environmental challenges under the context of climate resilience.

How to cite: Yang Hung, C. Y., Chen, Y. J., Chuang, W. C., and Tung, C. P.: Developing a Life Cycle Assessment Framework with Nature-based Solutions for Carbon Footprint Management in Irrigation Infrastructure, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2451, https://doi.org/10.5194/egusphere-egu25-2451, 2025.

ATMO-ACCESS is a pilot project funded under the Horizon 2020 program (April 2021–October 2025) that addresses the needs of distributed atmospheric research infrastructures (RIs), including ICOS (Integrated Carbon Observing System), ACTRIS (Aerosol, Clouds, and Trace Gases Research Infrastructure), and IAGOS (In-flight Global Observing System). The project provides effective and convenient access to leading European atmospheric research facilities, including fixed monitoring stations, mobile observation platforms, simulation chambers, and central laboratories. It also offers virtual access to innovative cross-RI digital and training services.

These access opportunities are utilized by research communities worldwide to conduct experiments, evaluate instruments, and analyze data, ultimately advancing scientific knowledge and technological development.

Now in its final stage, ATMO-ACCESS is reviewing its main outcomes. The presentation will highlight how demand for access to atmospheric research facilities is shifting—from physical access to more hybrid and virtual modes,  It will also discuss how transnational access projects can support both research and innovation and illustrate how access programs are used by the private sector or by international organization outside the academics.  

Historically, access projects have been funded through short-term EU initiatives. However, findings from ATMO-ACCESS underscore the need for greater collaboration among funding agencies across Europe and beyond. Such cooperation within Europe and extended at international level is essential to establish more sustainable access programs that benefit the broader research community.

How to cite: Laj, P. and Philippin, S.: ATMO-ACCESS: Why Do We Need a Sustainable Access Program for Atmospheric Research?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3748, https://doi.org/10.5194/egusphere-egu25-3748, 2025.

EGU25-4820 | Posters on site | ERE6.2

Building the Future of Biodiversity: Italy's National Biodiversity Future Center (NBFC) Initiative 

Donatella Spano, Carlo Calfapietra, Massimo Labra, Alberto Di Minin, Simonetta Frachetti, Gianluca Sarà, Maria Chiara Chiantore, Gian Marco Luna, Lorena Rebecchi, Francesco Frati, Maria Chiara Pastore, Andrea Galimberti, Hellas Cena, Gloria Bertoli, Isabella Saggio, Luigi Bubacco, Riccardo Coratella, Simone Mereu, and Giuseppe Brundu

This presentation provides an overview of a recent initiative and large investment in biodiversity undertaken in Italy. It focuses on establishing the Italian National Biodiversity Future Center (NBFC), the first National Research and Innovation Center dedicated to biodiversity, funded through European Union funds—NextGenerationEU. The NBFC includes key actions to monitor biodiversity, enhance conservation efforts, restore ecosystems, and value terrestrial, marine, and urban biodiversity. To deal with such a complex roadmap, the NBFC is designed following the Hub&Spoke model. It comprises 6 thematic Spokes dedicated to the sea, land and wetlands, and cities, with two crosscutting spokes dedicated respectively to training, communication, knowledge sharing, innovation, and policies through international connections. A primary objective is to encourage data sharing among various institutions, organizations, and countries to foster international collaboration in biodiversity protection. The NBFC is working to create a national digital platform for data analysis and biodiversity informatics, as well as collecting biodiversity data and acting as a digital twin for monitoring and conservation. This digital platform will connect biodiversity to ecosystem functions and services. This multilevel digital platform is a vital resource for the national and international scientific community, policymakers, and organizations responsible for protecting biological diversity in various environmental contexts. All actions undertaken by the NBFC are based on the Nature-based Solutions approach, providing a wide range of options for biodiversity restoration and management. Additionally, Citizen Science initiatives contribute to the NBFC's objectives by raising public awareness about the need to understand, monitor, conserve, and restore biodiversity. The NBFC's activities also aim to promote human health and well-being. In line with the One Health approach, healthy ecosystems are essential for resilience to diseases, food security, and improved quality of life. Through this initiative, Italy aims to strengthen its commitment to safeguarding biodiversity while promoting sustainable development and ecological resilience.

How to cite: Spano, D., Calfapietra, C., Labra, M., Di Minin, A., Frachetti, S., Sarà, G., Chiantore, M. C., Luna, G. M., Rebecchi, L., Frati, F., Pastore, M. C., Galimberti, A., Cena, H., Bertoli, G., Saggio, I., Bubacco, L., Coratella, R., Mereu, S., and Brundu, G.: Building the Future of Biodiversity: Italy's National Biodiversity Future Center (NBFC) Initiative, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4820, https://doi.org/10.5194/egusphere-egu25-4820, 2025.

EGU25-7674 | Orals | ERE6.2

The Ecological Monitoring System of Australia – standardised methods to track environmental change 

Sally O'Neill, Katie Irvine, Andrew Tokmakoff, Ashley Leedman, Jacqui DeChazal, Amelia Cook, and Ben Sparrow

The Australian Government makes significant investments to improve the stewardship of Australia's environment and the sustainable management of natural resources. On-ground actions by natural resource management (NRM) practitioners aim to improve or restore natural ecosystems and the diverse species they support, including threatened and unique taxa. Ideally, government investments are directed towards highly effective activities that result in positive conservation outcomes. Quality scientific data is critical not only to improve our understanding of the effectiveness of funded actions and their impact on species and ecosystems, but also to track climate-driven change, and enable policy-makers to make informed decisions. 

The Ecological Monitoring System of Australia (EMSA) is a collaboration between the Terrestrial Ecosystem Research Network (TERN) and the Australian Government Department of Climate Change, Energy, the Environment and Water (DCCEEW). EMSA provides the infrastructure, tools and resources to support NRM data collection, analysis, and evaluation, meeting the national requirement for a streamlined, consistent, automated, and robust ecological monitoring system.

EMSA builds on TERN's history as Australia’s terrestrial ecosystem observatory. EMSA’s consistent standardised observation methods provide on-ground practitioners with a modular suite of standardised survey protocols, comprehensive instructions manuals, a field data collection app, and centralised data management and storage system for the Australian Government's Biodiversity Data Repository. Ongoing support is provided via a help desk, community of practice, training and outreach activities.

The 24 EMSA modules include standardised methods for establishing plots, collecting landscape, soil, disturbance, vegetation community and floristic information, field vouchers, leaf tissue samples, and photopoints. Additional modules can be incorporated to target terrestrial fauna, pest fauna, and invertebrates through direct and indirect observation, camera trapping and acoustic monitoring. Modules are available to capture management activities, the severity of fire, and changes to tree condition and recruitment. Most modules offer multiple standardised options, depending on the detail required for the project. The field collection app is paired with an instruction manual and is written for entry to mid-level field ecologists and field practitioners.

EMSA is being delivered across Australia by partners funded under the Natural Heritage Trust. It is also encouraged for other NRM investment programs and is being considered for other future Australian Government programs. As a result, an Australian-wide network is being created, generating invaluable, science-rich data and improving our understanding of ecosystem restoration, biodiversity conservation, and climate change impacts, and supporting our planning, decision-making and reporting of investment programs Whilst developed for the Australian landscape, the EMSA model is adaptable globally.

How to cite: O'Neill, S., Irvine, K., Tokmakoff, A., Leedman, A., DeChazal, J., Cook, A., and Sparrow, B.: The Ecological Monitoring System of Australia – standardised methods to track environmental change, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7674, https://doi.org/10.5194/egusphere-egu25-7674, 2025.

EGU25-12915 | Orals | ERE6.2

eLTER Standard Observations: A holistic framework for integrated long-term environmental monitoring 

Steffen Zacharias, Jaana Bäck, and Michael Mirtl

The European Long-Term, critical zone and socio-ecologicalEcosystem Research Infrastructure (eLTER RI) has been developed to provide a continental-scale site-based network for the observation, understanding, and addressing of critical ecological, geochemical, and socio-ecological challenges. A cornerstone of this initiative is the implementation of the eLTER Standard Observations, which constitutes a harmonised framework for the collection and analysis of long-term environmental data across diverse ecosystems.

These observations are characterised by a multidisciplinary approach, integrating biological, hydrological, geochemical, climatic, soil-related, and socio-economic variables and parameters. Key areas of focus include biodiversity, primary production, water quality, nutrient cycling, carbon storage, and climate dynamics. The standardisation of the methodology ensures the comparability of data across sites, regions, and timescales, thereby enabling robust analyses of ecosystem dynamics and human impacts.

The eLTER Standard Observations (SOs) are closely aligned with the concepts of Essential Variables (EVs), encompassing a wide range of critical environmental parameters necessary for understanding ecosystem dynamics. SOs are designed to integrate elements of e.g. Essential Climate Variables (ECVs), Essential Biodiversity Variables (EBVs), and Essential Socio-Economic Variables (ESVs), ensuring a comprehensive approach to environmental monitoring. The SOs provide the fundamental data necessary to track key processes, assess ecosystem health, and understand human-nature interactions across various scales. By harmonising data collection and focusing on long-term monitoring, the SOs contribute to the global framework of Essential Variables, fostering comparability and supporting evidence-based decision-making.

The presentation will outline the scope, methodology, and significance of the eLTER Standard Observations with respect to simultaneously covering existing EV concepts. It will highlight their role in addressing global challenges such as climate change, biodiversity loss, and sustainable resource management, emphasizing their contribution to integrative ecosystem research.

How to cite: Zacharias, S., Bäck, J., and Mirtl, M.: eLTER Standard Observations: A holistic framework for integrated long-term environmental monitoring, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12915, https://doi.org/10.5194/egusphere-egu25-12915, 2025.

EGU25-12990 | Posters on site | ERE6.2

Biodiversity Knowledge Hub: Addressing the impacts of environmental change by linking Research Infrastructures, Global Aggregators and community Networks 

Christos Arvanatidis, Lyubomir Penev, Joaquin López Lérida, Cristina Huertas Olivares, Antonio José Sáenz Albanés, Alberto Basset, Sara Montinaro, Lucia Vaira, Nikos Minadakis, Michalis Griniezakis, and Julio López Paneque

Access to reliable information and FAIR compliant data is essential in understanding and addressing the impacts of environmental change on biodiversity and ecosystems. However, these resources are often fragmented and their combined use for delivering integrative knowledge to meet the above research challenge is difficult. The BiCIKL project (Biodiversity Community Integrated Knowledge Library) showcases the transformative potential of interdisciplinary collaboration in addressing biodiversity and climate research challenges. By integrating biodiversity data from research infrastructures, scientific repositories, and expert communities, BiCIKL has bridged the gap between fragmented knowledge systems and actionable insights for conservation and resilience.

A key achievement of BiCIKL is the Biodiversity Knowledge Hub (BKH), an innovative platform enabling seamless access to biodiversity data, tools, and workflows. The BKH fosters interoperability between diverse resources, empowering researchers, policymakers, and practitioners to make data-driven decisions that support biodiversity preservation and climate adaptation. This platform exemplifies open science principles and facilitates long-term, scalable solutions that support ongoing collaboration, innovation and resilience in biodiversity research and management.

Through its collaborative approach, BiCIKL has advanced biodiversity informatics by demonstrating best practices in data integration, capacity building, and stakeholder engagement. This positions BiCIKL as a benchmark for future efforts to harmonize biodiversity and climate resilience initiatives globally, exemplifying how interoperability and harmonized standards can transform the accessibility and utility of biodiversity data. The hub offers tailored tools that cater to a wide spectrum of users, from academic researchers conducting advanced analytics to policymakers seeking actionable insights for sustainable development.

BKH’s modular design allows for continuous expansion and adaptation, ensuring its relevance in addressing emerging challenges in biodiversity and climate resilience. By fostering active stakeholder engagement, BiCIKL has cultivated a thriving community of practice, ensuring the long-term sustainability and growth of its initiatives

This presentation will outline the methodologies and technologies contributing to BKH, emphasizing its role as a pioneering model for integrated biodiversity knowledge and action.

How to cite: Arvanatidis, C., Penev, L., López Lérida, J., Huertas Olivares, C., Sáenz Albanés, A. J., Basset, A., Montinaro, S., Vaira, L., Minadakis, N., Griniezakis, M., and López Paneque, J.: Biodiversity Knowledge Hub: Addressing the impacts of environmental change by linking Research Infrastructures, Global Aggregators and community Networks, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12990, https://doi.org/10.5194/egusphere-egu25-12990, 2025.

EGU25-13041 | ECS | Orals | ERE6.2

Learning from the European Experiences: Representativity on a Global Level 

Thomas Ohnemus and Michael Mirtl

The distributed Integrated European Long-Term Ecosystem, critical zone and socio-ecological Research Infrastructure (eLTER RI) is one of six partners of the Global Ecosystem Research Infrastructure (GERI). eLTER RI comprises ecosystem research sites and socio-ecological research platforms for exemplary research covering major European environmental, social and economic gradients. In a holistic approach, the in-situ facilities are designed for standardized observation of the five ecosystem spheres – socio-econosphere, atmosphere, hydrosphere, geosphere and biosphere. To identify gaps and to optimize the spatial distribution of in-situ facilities within eLTER RI we conducted analyses of representativity. These analyses reveal under-, well or overrepresented conditions and locations. However, these current conditions shift dramatically due to Global Change. Therefore, we additionally investigated the suitability of eLTER RI to address land use change and climate change features, i.e. the fitness for future.

We identified three distinct geospatial gaps: the Iberian Gap, the Eastern Gap, and the Nordic Gap. These gaps resulted mainly from the underrepresentation of agricultural lands, regions with low economic density, mesic and dry regions as well as the Mediterranean, Continental and Boreal biogeoregions. The patterns of underrepresentation appeared to be driven by access to funding resources and the regional research history. Several sites that responded to the survey but do currently not fulfil the infrastructural requirements of the eLTER RI bear potential to contribute to gap closure. Additionally, incorporating research facilities from other research infrastructures or monitoring networks into the eLTER RI could cost-efficiently counteract gaps. Regarding the fitness for future, eLTER RI covers all facets of emerging research challenges, but is spatially biased. Gaps that were assumed to be consistent for a variety of potential futures manifested in the Southern Iberian Peninsula, Poland, Finland, Sweden and Norway.

This work demonstrated the power of geospatial representativity analyses to investigate spatial biases and to inform strategic network development on the European continental scale. Consequently, we additionally harness this power to investigate the spatial distribution of the GERI initiative, which strives to better understand the function and change of indicator ecosystems across global biomes. To that end, GERI aims to support excellent science that can also inform political and managerial decision-making regarding grand societal challenges. A fully functioning GERI shall deliver harmonized data, foster international partnerships and enable new understandings of global ecological processes—stretching across continents, decades, and ecological disciplines. Therefore, the collective coverage of global ecosystems through the physical networks of SAEON (Z.A.), TERN (AUS), NEON (USA), CERN (China), as well as ICOS and eLTER RI in Europe is of high interest. As first analysis we present a global scale coverage of GERI-associated in-situ facilities regarding climatic zones.

How to cite: Ohnemus, T. and Mirtl, M.: Learning from the European Experiences: Representativity on a Global Level, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13041, https://doi.org/10.5194/egusphere-egu25-13041, 2025.

The forest landscape is of global importance for net radiative forcing. As the world warms, feedbacks within the ecosystems alter greenhouse gas (GHG) balances. Coordinated observations of GHG fluxes and concentrations, and of more chemically active species, as well as variables describing the ecosystem, are essential for understanding and prediction of feedbacks. ICOS (Integrated Carbon Observation System), ACTRIS (Aerosol, Clouds and Trace Gas Research Infrastructure) and SITES (Swedish Infrastructure for Ecosystem Science) have already provided >10 years of data for open science. These measurements on the carbon cycle, air quality, and ecosystem behavior already provide key information for quantifying GHG emissions and sinks, and investigating feedbacks under a changing climate. ACTRIS Sweden, ICOS Sweden and SITES have developed a strategic plan for enhanced cooperation. This will better address the global challenge of understanding ecosystem influences on GHG fluxes as the climate warms, as well as the interplay of physical and chemical properties of the atmosphere on ecosystems.

 

Before summarizing that plan for deeper cooperation, it is worth noting some more about these three national networks. ICOS and ACTRIS are already ERIC RIs and SITES is involved in efforts to establish eLTER (Integrated European Long-Term Ecosystem, Critical Zone and Socio-Ecological Research Infrastructure) as an ERIC RI as well. The three national RIs are active partners within their respective ERIC consortia and collaborate with other RIs in the ESFRI environment and climate domain. All stations and the FAIR data they provide are widely used within research, earth system observation, education (students, PhD, post docs), and as test sites for new instruments and methods within academia and private-sector companies. The stations of the three RIs are also incorporated into the Copernicus services. The management structure of the RIs are closely related to developments in earth observation at European and international levels.

 

The strategic plan for enhanced cooperation between the three national RIs has a set of eight short term goals that should be achieved in the next 2-3 years. These include further enhancing co-location of measurements, integration of scientific leadership, as well as coordination of tools for accessing both the field sites and available data. This enhanced cooperation between the national networks of ACTRIS, ICOS and SITES also aims at five long terms goals.

 

  • continuity of high-quality services
  • strategic collaboration
  • organizational optimization
  • increased usage across our RIs
  • fostering innovation

 

As a result of the enhanced cooperation, the RIs will achieve a new level of collaboration in observation systems for atmospheric pollution, including the effects of this pollution and climate change on ecosystems. Joint approaches to strategic development and outreach will further maximize synergies between these complementary infrastructures, giving ACTRIS, ICOS and SITES a more central, coordinated role in supporting Earth system science, and societal decision-making in the context of the UN Sustainable Development Goals.

How to cite: Krejci, R., Arnold, T., Holst, J., and Swietlicki, E.: Addressing research challenges of environmental change at the global scale via Research Infrastructures collaboration and alignment, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13250, https://doi.org/10.5194/egusphere-egu25-13250, 2025.

EGU25-13612 | ECS | Orals | ERE6.2

Towards Globally Harmonized Environmental Datasets: a Proof of Concept Using Ecological Drought Data and the Global Ecosystem Research Infrastructure (GERI) Framework 

Krutika Deshpande, Cedric Hagen, Tommy Bornman, Leo Chiloane, Gregor Feig, Elisa Girola, Siddeswara Guru, Christine Laney, Henry Loescher, Michael Mirtl, Beryl Morris, Paula Mabee, Emmanuel Salmon, Michael SanClements, Benjamin Ruddell, Pamela Sullivan, Melinda Smith, Werner Kutsch, Xiubo Yu, and Steffen Zacharias

Global environmental challenges, such as climate change, transcend international borders, requiring a unified approach to data management and analysis. The Global Ecosystem Research Infrastructure (GERI) was founded to address this need, building relationships and establishing data sharing practices among six of the largest ecosystem research infrastructures in the world. Data harmonization is required to standardize and ingest data products from these infrastructures into a findable, accessible, interoperable, reusable (FAIR) global dataset. Harmonized global data can improve existing global climate models and inform environmental research studies. Here, we present challenges involved in data harmonization and progress to date resulting from a U.S. National Science Foundation AccelNet award. This GERI-affiliated AccelNet project focuses on harmonizing ecological drought data collected by different countries and establishing a broader network-of-networks for pursuing ambitious global-scale environmental science research. We describe the analytical pipelines and the philosophical decisions made in designing the GERI framework, as well as some of the challenges and lessons learned along the way. We also present the initial harmonized drought data products, exploring how environmental variables like soil moisture and temperature vary across the world. Future work will be focused in two areas. First, working with our colleagues at DroughtNet and the International Drought Experiment, we will further explore the implications of these global harmonized drought data. Second, we will begin global data harmonization efforts for new data products related to other research areas, primarily led by the GERI early career researcher working group.

How to cite: Deshpande, K., Hagen, C., Bornman, T., Chiloane, L., Feig, G., Girola, E., Guru, S., Laney, C., Loescher, H., Mirtl, M., Morris, B., Mabee, P., Salmon, E., SanClements, M., Ruddell, B., Sullivan, P., Smith, M., Kutsch, W., Yu, X., and Zacharias, S.: Towards Globally Harmonized Environmental Datasets: a Proof of Concept Using Ecological Drought Data and the Global Ecosystem Research Infrastructure (GERI) Framework, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13612, https://doi.org/10.5194/egusphere-egu25-13612, 2025.

EGU25-14518 | ECS | Orals | ERE6.2

Assessing coastal ecosystem impacts of sea-level rise at the global scale via research infrastructure alignment 

Madeline Goddard, Vicki Bennion, Catherine Lovelock, and Neil Saintilan

TERN Australia, a GERI member in the southern hemisphere, produces systematically collected continental-scale time-series ecosystem data. These data are invaluable to a myriad of global models and sustainability reporting and help enable broader cross-continental ecological research. This presentation focuses on the challenges of federating recently introduced sea-level coastal ecosystem research infrastructure for future global impact. Understanding the vulnerability of vegetated coastal habitats is essential - they support biodiversity, filter pollutants, capture sediments and reduce coastal erosion and storm damage. They also on average sequester more carbon per unit area than terrestrial forest and maintain significant sedimentary carbon stocks. Australia has one of the longest coastlines in the world and to date, has over 300 surface elevation table (SET) instruments monitoring sea level rise impacts on coastal wetlands. SETs present a cost-effective methodology, collecting long term empirical datasets that may be integrated into remote sensed data. TERN aims ensuring all Australian SET operators adhere to ‘global standard’ for monitoring and data curation protocols so that the data can be harmonised with that of the 20-30 other countries, including other GERI members, to form the global SET network, systematically assessing and predicting coastal wetland responses to accelerating sea-level rise in the decades ahead.

How to cite: Goddard, M., Bennion, V., Lovelock, C., and Saintilan, N.: Assessing coastal ecosystem impacts of sea-level rise at the global scale via research infrastructure alignment, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14518, https://doi.org/10.5194/egusphere-egu25-14518, 2025.

EGU25-14534 | Posters on site | ERE6.2

Harmonizing Stable Isotope Data in Australia: The isotopes.au Platform for Enhanced Data Sharing and Collaboration 

Nina Welti, Wayne Noble, Geoff Fraser, Lian Flick, Christoph Gerber, Steph Hawkins, Cath Hughes, Fabian Kohlmann, Tim Stobaus, Axel Suckow, Moritz Theile, Kathryn Waltenberg, and Xinyan Zhang

Large volumes of isotope data have been collected across many scales and for a diverse range of purposes. From international and national scale monitoring and measurement efforts to short term assessments such as academic projects and citizen science efforts.  These all continue to contribute to creating significant data assets. Yet, the difficulty extracting and integrating these data resources into workflows limits the potential value.  Data collection, management and analysis efforts are siloed by funding models and contractual agreements, resulting in a fragmented data landscape.

In Australia, environmental isotope data in environmental media, such as water, soil, rocks, plants and animals, have been accumulated over many decades in public organisations including federal and state government agencies and universities. Federal science agencies are key custodians of such data and already disseminates data through established organizational channels, such as the CSIRO Data Access Portal (DAP) and Geoscience Australia's Portal Core. However there remains an ambiguity about an institutional mandate for collecting and disseminating data, leading to a lack of coordination and sharing.

We present the process of harmonizing publicly held stable isotope data from Australian public organisations into a coherent user experience. Data across multiple Australian organisations has been harmonised through an interoperable architecture and common ontology, co-developed with wide consultation across the stable isotope community in Australia. This includes implementing robust data collection strategies, ensuring data quality control, and transparent data stewardship governance.

Existing data silos of big data repositories were translated in an aligned manner through a flat ontology, so data can be gathered and reused across different isotopic data sources. This was done while maintaining FAIR standards and preserving the autonomy of source institutions' internal data structures and governance systems. The isotopes.au platform and ontology are presented as a bottom-up solution with an additive architecture to be flexible across multiple future applications.

The goals of this multi-institutional effort are to create greater usability and availability of publicly-held data, increase collaboration of research infrastructure, and realise greater value from public data.  This supports good outcomes for both private and public usage. The next step is to expand the network of connected data sources and facilitate development of modelling applications supported by isotopes.au.

By leveraging big data through platforms like isotopes.au and fostering international collaboration, Australia and Europe can work together to establish robust and efficient data sharing mechanisms

How to cite: Welti, N., Noble, W., Fraser, G., Flick, L., Gerber, C., Hawkins, S., Hughes, C., Kohlmann, F., Stobaus, T., Suckow, A., Theile, M., Waltenberg, K., and Zhang, X.: Harmonizing Stable Isotope Data in Australia: The isotopes.au Platform for Enhanced Data Sharing and Collaboration, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14534, https://doi.org/10.5194/egusphere-egu25-14534, 2025.

EGU25-14907 | Orals | ERE6.2

EcoPlots - The data Integration platform for systematic site-based surveys 

Siddeswara Guru, Javier Sanchez Gonzalez, Avinash Chandra, Arun Singh Ramesh, Junrong Yu, and Gerhard Weis

Harmonised ecology systematic survey site-based data is critical for trans-geography and trans-disciplinary research. However, integrating site-based survey data from multiple sources remains challenging due to the lack of data representation and exchange standards. 

TERN, Australia’s trusted name in research infrastructure development, has developed EcoPlots to integrate site-based survey data from multiple sources and provide integrated search and access capabilities. EcoPlots map source data to a standard information model and allow users to search based on multiple regions, data sources, methods used in the data collection, feature types, parameters, and observation date ranges. 

Users can also search for species, filter parameters and attributes with exact values and ranges. They can download data in multiple formats, including a comprehensive ontology-based CSV file format, simple CSV, and GeoJSON, which contains all observations related to a site. In addition, users can mint DOIs for their search outputs to improve the reusability of data. In Australia, EcoPlots has enabled the integration of site-based survey data across research infrastructure projects, academia, and government agencies.

How to cite: Guru, S., Sanchez Gonzalez, J., Chandra, A., Ramesh, A. S., Yu, J., and Weis, G.: EcoPlots - The data Integration platform for systematic site-based surveys, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14907, https://doi.org/10.5194/egusphere-egu25-14907, 2025.

EGU25-16083 | Posters on site | ERE6.2

Simplifying cost calculations for eLTER sites and platforms: A flexible web application for site managers  

Allan Souza, Syed Ashraful Alam, Terhi Rasilo, Steffen Zacharias, and Jaana Bäck

The eLTER-SO-Costs web application is a specialized tool designed to assist the eLTER (integrated European Long-Term Ecosystem, critical zone and socio-ecological Research) community in estimating the costs associated with upgrading and operating standard observations (SOs) across various eLTER sites. It provides a flexible and efficient approach to cost estimation by tailoring calculations to specific site characteristics, ensuring that cost assessments are relevant and accurate. The tool considers key factors such as the site category, habitat types, focus spheres, and the potential for co-location with other research infrastructures, all of which influence the costs. The application is designed to be highly adaptable, allowing users to customize the output according to specific needs and exclude or adjust certain predefined cost elements based on the unique conditions of their sites or platforms. The core functionality of the application allows users to input unique site-specific data and receive an automated, detailed annual cost breakdown for SOs. The eLTER-SO-Costs facilitates financial planning, enabling eLTER site managers to optimize their eLTER site management, reducing the time and effort traditionally spent on manual cost calculations, democratizing access to essential financial data for the broader eLTER community. The tool's user-friendly interface ensures that site managers and researchers, even those without expertise in cost analysis, can efficiently plan for the long-term sustainability of their sites while meeting the scientific and operational demands of ecological monitoring.  

How to cite: Souza, A., Alam, S. A., Rasilo, T., Zacharias, S., and Bäck, J.: Simplifying cost calculations for eLTER sites and platforms: A flexible web application for site managers , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16083, https://doi.org/10.5194/egusphere-egu25-16083, 2025.

EGU25-20665 * | Orals | ERE6.2 | Highlight

Investigating sustainability across scales through social-ecological land-use studies in LTSER platforms 

Veronika Gaube, Claudine Egger, Bastian Bertsch-Hörmann, and Benedikt Grammer

Sustainability challenges are related to socio-ecological interactions that take place at different spatial and temporal scales. Processes at different scales are interlinked, so that place-based research - like the LT(S)ER approach in eLTER - needs to be embedded in larger, often global, contexts. This is all the more important today, as increasing geopolitical tensions, international conflicts and the increasingly frequent and severe effects of global warming are pushing the world towards a "divided world" scenario. For example, changing environmental conditions due to climate heating but also land-use change, pose major threats to biodiversity and ecosystems. Changes in their biophysical and socio-economic framework will force land users to rethink and adapt their land management strategies in terms of land cover and land-use intensity. To link societal and environmental drivers of land use change, we developed the land-use agent-based model (ABM) SECLAND. The model’s farm agents represent real-world actors who make decisions in pursuit of well-being, intrinsic motivation and global socioeconomic and political drivers for decision-making influencing their preferences for certain land-use strategies. We will present new simulations for the LTSER (Long-term socio-ecological research) region Eisenwurzen in Austria, for which we calibrated the model with quantitative census data, supplemented by qualitative data from interviews and workshops with stakeholders to represent the specific conditions of the study region. Model simulations produce spatially explicit parcel-level land use maps. Previous land-use trajectories proposed strong shifts toward organic and extensive agriculture as well as forest transition as result of (grass-) land abandonment. We refine these forecasts by focusing on farmers’ perception of extreme events as climate change threats and evaluate the effects of early climate change adaptation measures on future land management. Based on this research example we will discuss the power of such models for transformative research, linking the biophysical processes of land use change to actors, institutions and power relations. Such social ecology methods and tools are important for exploring the integration of social and natural sciences in studying the sustainability of globally embedded socio-ecological systems. The investigation of social-ecological research in an RI such as eLTER can thus make a crucial contribution to the integration of local, actor-centred and participatory research carried out in LTSER regions into larger-scale models and assessments.

How to cite: Gaube, V., Egger, C., Bertsch-Hörmann, B., and Grammer, B.: Investigating sustainability across scales through social-ecological land-use studies in LTSER platforms, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20665, https://doi.org/10.5194/egusphere-egu25-20665, 2025.

EGU25-21300 | Orals | ERE6.2

The Global Ecosystem Research Infrastructure (GERI): How we got here?, Where are we going? 

Henry W. Loescher, Michael SanClements, Steffen Zacharias, Tommy Bornman, Gregor Feig, and Paula Mabee

Recognizing that contemporary environmental challenges transcend geopolitical boundaries, the Global Ecosystem Research Infrastructure (GERI) was formed to address the nature and magnitude of these challenges through cross-border global perspectives and collaborations.  GERI brings together six major ecosystem research infrastructures (RIs) (i.e., SAEON in South Africa, TERN in Australia, CERN in China, NEON in the USA, and ICOS and eLTER in Europe) to federate the programmatic work needed for concerted operation, collaborations, and the provisioning of interoperable data and services.  Here, we present the historical activities that brought these RIs together, establishing a structured governance, and current overview of GERIs data harmonization and common services.  We will also present current programmatic challenges as GERI continues to develop internationally and seek community input and involvement.

How to cite: Loescher, H. W., SanClements, M., Zacharias, S., Bornman, T., Feig, G., and Mabee, P.: The Global Ecosystem Research Infrastructure (GERI): How we got here?, Where are we going?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21300, https://doi.org/10.5194/egusphere-egu25-21300, 2025.

Identification of source rocks bearing helium generation potential is essential to construct a robust play fairway for natural helium exploration. The main source rock for helium generation are widely accepted as granitic or metamorphic basement rocks of cratons while some researchers suggest that hydrocarbon source rocks and sediments might also generate helium. One of the most critical implications for potential zones is the presence of radioactivity as He generation is sourced from the alpha decay of 232Th, 238U, and 235U. Thus, more He generation means more decay, characterised by increasing radioactive heat. In addition, distinguishing heavy thorium minerals as clay types by 232Th-40K cross-plots could also indicate potential zones. Therefore, measuring and assessing the 232Th-238U-40K levels play a critical role in any region for natural helium exploration.

This study brings forward well log interpretation approach as one of the transferable methods from the oil and gas industry into natural He exploration by examining the 232Th-238U-40K concentration logs, known as SGR logs, which are generally neglected or overlooked although they provide numerous benefits for subsurface evaluation.

Based on the methodology 2 main research questions emerge for this study to answer;

  • Can sediments and hydrocarbon source rocks might generate He or contribute to the He generation process?
  • Can SGR Logs provide a robust methodology for detection of potential He generating intervals in sedimentary successions?

To answer these questions, Early and Mid-Triassic sediments from the Northern Arabian Plate are selected as a case study. Recently unlocked Mid-Triassic hydrocarbon play, including source rocks, and CO2 / N2 readings on gas chromatography of nearby wells make the region unique and a perfect study area to test the hypothesis. Radiogenic heat generations (A) have been calculated using the equation below to track radioactivity levels.

A = 0.01 p (9.52 238U + 2.56 232Th + 3.48 40K)

A; radiogenic heat (μWm–3),

p; rock density (g/cm3),

238U, 232Th, 40K; Uranium 238U (ppm); Thorium 232Th (ppm); potassium 40K (%)

Regarding the observations, a 1-15 m. thick, theoretical He generation zone has been detected in the shales of the Early Triassic succession. A consistent significant peak in radiogenic heat levels reaching 4 μWm–3 coincide with rapid increases in calculated He log and heavy thorium minerals content. Additionally, shales are represented by as high 232Th-238U levels as granitic basements. A thickness map of potential He generation zone demonstrates that the zone gets thinner towards ESE at where large fault zones dominate the regional geology.

As a conclusion, the findings of this study suggest that sediments might generate natural He and potential zones might be identified by the help of SGR logs. The results can also shed light on the He generation potential of Triassic sediments deposited in the other regions of the Arabian Plate. Moreover, the proposed workflow can be applied for any region or rock type if the interval of interest is covered by 232Th-238U-40K concentration logs.

How to cite: Uyanik, A.: Can Sediments Generate Helium? Implications from 232Th-238U-40K Concentration Logs from the Northern Arabian Plate, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1138, https://doi.org/10.5194/egusphere-egu25-1138, 2025.

EGU25-1857 | ECS | Orals | GD6.1

A Multi-Scale Framework for Evaluating Hydrogen Generation in Serpentinization Settings 

Rodolfo Christiansen, Mohamed Sobh, Nicolas Saspiturry, and Gerald Gabriel

This study presents a versatile methodological framework, implemented as a Python-based tool called PoNHy (Potential for Natural Hydrogen), designed to assess hydrogen generation in serpentinization environments using geophysical and laboratory data. As a practical application, the approach robustness is demonstrated in the Mauleon Basin localized in the north-western Pyrenees, where extensive data availability facilitates detailed analyses and validation. The workflow begins with a thorough assessment of key petrophysical properties such as density, magnetic susceptibility, and thermal conductivity. These properties guide the interpretation of underlying geological structures and help refining the initial subsurface models. Building on this foundation, gravity and magnetic data are inverted to determine the distribution and volume of source rocks, as well as their degree of serpentinization. Thermal modeling then delineates subsurface temperature regimes, which play a critical role in the serpentinization reactions and subsequent hydrogen production. To translate laboratory-derived hydrogen production rates into realistic field estimates, the framework integrates parameters from both lab experiments and field observations. Factors such as the water-to-rock ratio, fracture spacing, mineral composition, and specific surface area of reacting materials influence fluid flow, reaction rates, and the overall efficiency of hydrogen generation. By integrating these parameters alongside corrections for the degree of serpentinization, our new methodology provides a more accurate representation of subsurface conditions. This comprehensive integration yields hydrogen generation estimates that better reflect in situ conditions, ultimately improving our understanding of natural hydrogen volumes. Such insights are critical for subsequent transport models aimed at identifying potential reservoirs.

How to cite: Christiansen, R., Sobh, M., Saspiturry, N., and Gabriel, G.: A Multi-Scale Framework for Evaluating Hydrogen Generation in Serpentinization Settings, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1857, https://doi.org/10.5194/egusphere-egu25-1857, 2025.

EGU25-2570 | ECS | Orals | GD6.1

Alpine-type orogens are great sites for natural H2 exploration 

Frank Zwaan, Sascha Brune, Anne C. Glerum, Dylan A. Vasey, John B. Naliboff, Gianreto Manatschal, and Eric C. Gaucher

As the energy transition gathers steam, naturally occurring hydrogen gas (H2) generated by the serpentinization of mantle rocks is a highly promising sustainable alternative to fossil fuels. To undergo serpentinization, mantle rocks that are normally situated at great depth need to be brought closer to the surface by plate tectonics and other geodynamic processes. Here, they may react with water to be efficiently serpentinized and generate natural H2, which can accumulate in reservoirs as it migrates to the surface (as part of a natural H2 system).

Exploring natural H2 systems requires a solid understanding of their geodynamic history, which can be informed by numerical geodynamic modelling. Through such modelling we can trace how, when, and where mantle material enters the serpentinization window, as well as when active, large-scale faults penetrate exhumed mantle bodies allowing for water circulation, as well as serpentinization and H2 generation, to occur.

Our recent modelling of rifting and subsequent rift inversion (Zwaan et al., in press) shows that, although serpentinization-related natural H2 generation is a phenomenon best known from (magma-poor) rifted margins and oceanic spreading ridges, annual volumes of natural H2 generated during inversion may be up to 20 times higher than during rifting, due to the colder thermal regime in rift-inversion orogenic environments. Moreover, suitable reservoir rocks and seals required for natural H2 accumulations to form are readily available in rift-inversion orogens, whereas they may not be present when serpentinization occurs in deep marine continental rift or oceanic spreading settings.

Our model results thus provide a first-order motivation to turn to rift-inversion orogens for natural H2 exploration and are supported by indications of natural H2 generation in rift-inversion orogens such as the European Alps and Pyrenees.

REFERENCE CITED: Zwaan, F., Brune, S., Glerum, A.C., Vasey, D.A., Naliboff, J.B., Manatschal, G., Gaucher, E.C (in press). Rift-inversion orogens are potential hotspots for natural H2 generation. Science Advances. Link to preprint: https://doi.org/10.21203/rs.3.rs-3367317/v1

How to cite: Zwaan, F., Brune, S., Glerum, A. C., Vasey, D. A., Naliboff, J. B., Manatschal, G., and Gaucher, E. C.: Alpine-type orogens are great sites for natural H2 exploration, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2570, https://doi.org/10.5194/egusphere-egu25-2570, 2025.

EGU25-2903 | Posters on site | GD6.1

The importance of geodynamic settings and exploring for geothermal energy   

Philip Ball, Graham Banks, Mikenna Montgomery, Juan Carlos Afonso, and Vladimir Stroganov

Scaling up geothermal from a niche industry to a viable, global industry is important for all our collective decarbonization efforts. Here we explore the distribution of geothermal projects globally to understand where projects have been positioned to date. As a result of this global analysis, we recommend that future geothermal exploration and development be conducted using a Linnean-style classification system for geothermal entities. Hierarchical thinking and the pre-discovery exploration triangle will provide the technique for gaining the ‘big picture’ context about the location of the optimal geothermal plays and prospects.  It is further argued that the engineering approach used to complete a geothermal project significantly impacts the economics of the project, and that engineering should not be confused with play type, which at the highest level is either hydrothermal or petrothermal.

In this study we explore the distribution of Natural hydrothermal systems (NHS), Open loop Geothermal Systems (generically known EGS), and Closed Loop geothermal  systems (generically known CLG or AGS). Using the geodynamic model of Hasterock et al., (2022) our findings include an observation that there is little or no coherence to geothermal exploration to date. CLG/Closed Loop: Volcanic Arc systems (44%) EGS/Open Loop: Orogenic Belt systems (45%). Natural Hydrothermal: Volcanics Arc systems (51%). Our analysis is the first coherent global study of the geodynamic domain of geothermal projects. We observe that a better understanding of the internal variation within geodynamic domains and refined geodynamic models (paleo and present day) are necessary to improve the success of geothermal exploration. Furthermore, we find that identifying present day stress-state is important when planning wells and executing geothermal projects, and that higher resolution lithospheric models are needed to help understand the petrothermal and hydrothermal systems. Finally, further R&D is needed to help unlock geothermal exploration and drilling across the most prolific geodynamic settings.

How to cite: Ball, P., Banks, G., Montgomery, M., Afonso, J. C., and Stroganov, V.: The importance of geodynamic settings and exploring for geothermal energy  , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2903, https://doi.org/10.5194/egusphere-egu25-2903, 2025.

EGU25-3033 | ECS | Orals | GD6.1

Geometry and Kinematics of the Hormuz Salt in the United Arab Emirates: The Jebel Al Dhanna Salt Dome 

Moamen Ali, Mohammed Ali, and Hamda Alshehhi

The UAE government is actively exploring the use of Hormuz salt domes for large-scale hydrogen and hydrocarbon storage, aligning with its strategic goals for clean energy transition and decarbonization. A comprehensive understanding of the geometry, kinematics, and halokinetic phases of these Infra-Cambrian Hormuz salt structures is crucial to achieving this vision. This study focuses on the Jebel Al Dhanna salt dome, the only exposed salt dome in onshore Abu Dhabi. Utilizing three 3D seismic surveys and data from four boreholes, the research analyzes its morphology and evolution. The Jebel Al Dhanna salt dome exhibits an elliptical structure elongated in the N-S direction, with dimensions ranging from 2 to 2.8 km (E-W) and 3.2 to 4.2 km (N-S). The dome features irregular crests, steeply dipping flanks, and a series of hills rising approximately 110 m above sea level. Surrounding the dome is a pronounced rim syncline, resulting from the upward evacuation of Hormuz salt through the thick Phanerozoic stratigraphic succession, creating a discordant relationship with the dome structure. Salt withdrawal at Jebel Al Dhanna likely initiated in the Late Cretaceous, driven by the reactivation of inherited basement faults associated with ophiolite obduction onto the Arabian foreland. Halokinetic activity persisted through the Oligocene-Miocene, coinciding with the continent-continent collision of Central Iran and the Arabian Plate. The presence of tilted Upper Miocene and Quaternary strata around and within the Jebel Al Dhanna salt dome underscores continued salt evacuation to the present day. This research highlights the importance of salt tectonics for energy resource storage and provides valuable insights into fault-salt interactions, with significant implications for hydrocarbon exploration, energy security, and the UAE’s decarbonization initiatives.

How to cite: Ali, M., Ali, M., and Alshehhi, H.: Geometry and Kinematics of the Hormuz Salt in the United Arab Emirates: The Jebel Al Dhanna Salt Dome, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3033, https://doi.org/10.5194/egusphere-egu25-3033, 2025.

EGU25-3367 | Orals | GD6.1

Lithospheric thermal-rheological structure and shallow thermal response in eastern China 

Haonan Gan, Xiao Wang, Guiling Wang, Wei Zhang, Linxiao Xing, and Yu Zhang

Eastern China (EC) is located in the eastern margin of the Eurasian Plate and has been influenced by the subduction of the Izanagi and Pacific Plate since the Late Mesozoic, resulting in a large amount of tectonic-magmatic activities. After the India–Eurasia convergence, the topography of continental China changed from high-east-low-west to high-west-low-east. At present, the Bohai Bay Basin in EC mainly forms sedimentary basin-type geothermal system, and deep circulation-type geothermal systems mainly occur in southeast coastal China, with thermal springs widely distributed. In the northeastern China, Holocene volcanoes such as Changbaishan Volcano have been formed, together with many thermal springs exposed.

The genesis of shallow thermal anomalies is closely correlated with the thermal-rheological structure of the lithosphere. In this study, we comparatively analyzed the lithospheric thermal-rheological structures of different tectonic units in EC, such as the Bohai Bay Basin, the southeast coastal China, and the Changbaishan Volcano field. We revealed that under the influence of the Pacific tectonic domain, the lithospheric thermal structures differed significantly, and the temperatures at the same depth from high to low are the Changbaishan Volcano field, the Bohai Bay Basin and the southeast coastal China. The rheological structures are significantly weakened in the middle and lower crust in the presence of an intracrustal heat source. The shallow thermal anomalies in the three tectonic units are similar in that the reservoir temperatures are mainly in the range of 100-150°C, and the water sources are all meteoric water. The difference between shallow thermal anomalies corresponds to their lithospheric thermal-rheological structures. The geothermal systems in the sedimentary basin of the Bohai Bay Basin are characterized by wells with a geothermal reservoir depth of 3-5 km. The deep-circulation hydrothermal systems in southeast coastal China are characterized by springs with a circulation depth of 4-7 km, and the hydrothermal systems in the Changbaishan Volcano field are characterized by springs with a circulation depth of 4-5 km. The deep thermal-rheological structure influences the behavioral characterization of shallow thermal anomalies with respect to heat-accumulation patterns. When brittle-ductile transition depth greater than the circulation depth, magma chamber (or partial melting body) and fluid circulation systems are relatively independent, and mass transfer from the magma chamber to the geothermal system may not happen.

How to cite: Gan, H., Wang, X., Wang, G., Zhang, W., Xing, L., and Zhang, Y.: Lithospheric thermal-rheological structure and shallow thermal response in eastern China, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3367, https://doi.org/10.5194/egusphere-egu25-3367, 2025.

EGU25-3694 | ECS | Posters on site | GD6.1

The enigmatic role of cratons in Zn-Pb deposit formation during continental rifting 

Anne Glerum, Sascha Brune, Philipp Weis, Joseph M. Magnall, and Sarah A. Gleeson

The growing global demand for metal resources requires new discoveries of high-grade ore deposits. Known sediment-hosted clastic-dominated base metal deposits are found in failed continental rifts and the passive margins of successful rifts. Recent studies indicate that the majority of these Zn-Pb deposits are located near steps in lithospheric thickness (e.g., Hoggard et al., 2020), but a potential causal link between ore formation and craton edges remains elusive. However, numerical models have shown that a craton edge close enough to an incipient rift controls the direction of asymmetry of the rift system (Raghuram et al., 2023) and that asymmetric rifts are more favorable to deposit formation (Glerum et al., 2024). Understanding the large-scale controls of cratons on rift-related mineralizing processes, occurring on much smaller spatial and temporal scales, can thus help identify new areas for exploration.

To this end, we use the geodynamic code ASPECT (Kronbichler et al., 2012; Heister et al., 2017) coupled to the landscape evolution model FastScape (Braun and Willett, 2013; Neuharth et al., 2022) to model 2D rift systems from inception to break-up in the presence of a craton. We investigate the relationship between craton distance and favorable conditions for ore formation, i.e., those conditions where potential source rock, host rock, and fluid pathways co-occur. Our results show that cratons have a negative effect on ore formation in narrow asymmetric rifts, but a positive effect in wide rifts.

In a second step, we further investigate the hydrothermal ore-forming mechanisms by using potentially favorable geodynamic configurations from the ASPECT simulations as input for fluid flow modelling with CSMP++ (Weis et al., 2014; Rodríguez et al., 2021). This input comprises basin geometry, temperature, boundary heat flow and a permeability structure dependent on strain and strain rate. With a temperature- and salinity-dependent proxy of metal solubility in the basinal brines, we track the leaching, transport, and precipitation of metals. This cross-scale workflow allows us to identify those rifting scenarios with the highest metal enrichment potential.

 

References:
Braun and Willett, 2013. Geomorphology 180–181: 170–79. DOI: 10.1016/j.geomorph.2012.10.008.
Glerum et al., 2024. Solid Earth 15: 921-944. DOI: 10.5194/se-15-921-2024.
Heister et al., 2017. Geophys. J. Int. 210 (2): 833–51. DOI: 10.1093/gji/ggx195.
Hoggard et al., 2020. Nat. Geosci. 13 (7): 504–10. DOI: 10.1038/s41561-020-0593-2.
Kronbichler et al., 2012. Geophys. J. Int. 191 (1): 12–29. DOI: 10.1111/j.1365-246X.2012.05609.x.
Neuharth et al., 2022. Tectonics 41 (3): e2021TC007166. DOI: 10.1029/2021TC007166.
Raghuram et al., 2023. Geology 51:1077–1082. DOI: 10.1130/G51370.1.
Rodríguez et al., 2021. GCubed 22 (6). DOI: 10.1029/2020GC009453.
Weis et al., 2014. Geofluids 14, 347-371. DOI: 10.1111/gfl.12080.

How to cite: Glerum, A., Brune, S., Weis, P., Magnall, J. M., and Gleeson, S. A.: The enigmatic role of cratons in Zn-Pb deposit formation during continental rifting, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3694, https://doi.org/10.5194/egusphere-egu25-3694, 2025.

EGU25-4193 | ECS | Posters on site | GD6.1

Geodynamic controls on the geothermal potential in the Upper Rhine Graben, France-Germany: a multi-scale numerical modelling approach 

Alan J. Yu, Sascha Brune, Judith Bott, Anne C. Glerum, and Magdalena Scheck-Wenderoth

The Upper Rhine Graben (URG), situated along the border of France and Germany, is part of the intraplate European Cenozoic Rift System. The graben is widely recognized for its abundant geothermal resources, making it a key region for energy transition initiatives. However, the characterization of the URG’s geothermal potential remains poorly constrained due to its highly variable hydrothermal conditions and large observational gaps. Previous studies on fault criticality have often overlooked the role of historical plate movements, oversimplifying the intricate interactions that govern the thermal and structural evolution of the URG over the past ~40 million years.

Using the numerical geodynamic code ASPECT coupled with the landscape evolution code FastScape, we simulate the lithospheric-scale development of fault networks within the URG under geodynamically realistic stress and strain conditions. Our models incorporate various forms of structural and rheological heterogeneities inherited from the earlier Variscan Orogeny, along with a two-stage Cenozoic kinematic history involving rift-orthogonal extension followed by sinistral strike-slip. Preliminary results show the first-order impact of structural inheritance and divergence obliquity on strain localization, which shape the orientation, spacing, and strain rate of the resulting fault network. These results will lay the groundwork for subsequent basin-wide modelling with the thermo-hydro-mechanical code GOLEM, coupling geodynamically controlled basin development with heat and fluid flow simulations that involve shorter-term rock and fracture mechanics. Throughout all modelling stages, we compare our models with available geological and geophysical observations.

How to cite: Yu, A. J., Brune, S., Bott, J., Glerum, A. C., and Scheck-Wenderoth, M.: Geodynamic controls on the geothermal potential in the Upper Rhine Graben, France-Germany: a multi-scale numerical modelling approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4193, https://doi.org/10.5194/egusphere-egu25-4193, 2025.

EGU25-6373 | Orals | GD6.1

A petro-physical model for serpentinised mantle and origin of natural hydrogen in the Pyrenees 

Alexandra Robert, Sepideh Pajang, Frederic Mouthereau, Ajay Kumar, and Jean-Paul Callot

The relationships between the serpentinised continental mantle in orogens, its geophysical signature at depth and hydrogen seepages are poorly understood. A petro-physical modelling approach accounting for serpentinisation shows that a large domain of serpentinised mantle is present in the northern Pyrenees. The serpentinisation reached a maximum of 40% during the mid-Cretaceous rifting, according to the predicted temperature and pressure. Although high-temperature serpentinisation could have generated large quantify of hydrogen during the Mesozoic, the shallow and inactive faulting in Northern Pyrenees make this process unlikely to explain the entire serpentinisation inferred by petro-physical modelling. A combination of low-temperature alteration of mafic and ultramafic rocks in the North Pyrenean Zone, active normal faulting in the North Pyrenean Fault, accumulation in local traps and transport of H2-rich fluids along inactive but permeable fault may explain the hydrogen seepages observed today.

How to cite: Robert, A., Pajang, S., Mouthereau, F., Kumar, A., and Callot, J.-P.: A petro-physical model for serpentinised mantle and origin of natural hydrogen in the Pyrenees, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6373, https://doi.org/10.5194/egusphere-egu25-6373, 2025.

EGU25-7103 | ECS | Orals | GD6.1

The role of intra-salt heterogeneity on the internal and external geometry of salt bodies – a numerical modelling approach with applications for geo-storage 

Leonardo Pichel, Ritske Huismans, Thomas Theunissen, Sabine Delahaye, Alexandre Pichat, Jean-Paul Callot, and Naim Celini

Thick salt deposits occur in a wide range of sedimentary basins and orogens. They are associated with large and geometrically complex structures due to the inherent ability of salt to flow as a viscous fluid. Salt basins form major hydrocarbon provinces and are increasingly targeted for CO2/H2 storage and geothermal energy due to the unique physical properties of salt, its low viscosity, high thermal conductivity and impermeability. Despite considerable advances in understanding salt basins and salt tectonics, there is still a significant knowledge gap on the internal geometry of salt structures. We apply a novel, very-high resolution (20x50m)2D numerical modelling approach to simulate salt diapirism and minibasin formation for heterogenous, layered salt sequences. We test the effects of varying i) viscosity, ii) density, iii) thickness, and iv) stratigraphic arrangement of intra-salt layers on the kinematics, and the internal and external geometries of deformed salt bodies by using scaled material properties to simulate: i) weak pure halite, ii) less-weak impure halite, ii) strong and dense anhydrite-rich layers, and iv) very-weak K-Mg salts.

Our results show that salt sequences including an alternation of weak and less-weak layers with different viscosity and density produce major intra-salt strain partition and complexity characterized by highly convoluted folding, horizontal and vertical shearing, and preferential flow of the weaker, less-dense salt (pure halite) into the core of diapirs. The less-weak layers can eventually flow into the diapir crest but are generally disrupted by flow of the underlying weak layers and positioned towards the diapirs’ flanks where they become overturned. The most complex and convolute intra-salt geometries occur around the diapirs’ flanks when there is an abrupt internal shift of minibasin depocentres. Recumbent intra-salt folds are also common and associated with the development of secondary minibasins by diapir-fall. For models that include strong anhydrite-rich layers, there is a general decrease in the magnitude and complexity of diapirism, with these layers being passively folded by flow of the underlying weak salt and displaying only moderate to negligible flow onto diapirs and vertical stretching. These stronger layers become trapped underneath the base of diapirs and their associated minibasins where they typically form short-wavelength folds. For models that include very-weak and light K-Mg salt layers, there is an increase in rate of diapirism with rapid vertical shearing and stretching of the weak layers along the diapir’s flanks and sub-horizontal flow and recumbent folds along their crests. Varying the position of both very-weak and strong layers generates very contrasting internal and external diapir geometries. These results can aid in the characterization of the internal structures of deformed, diapiric salt bodies, which is critical for the use of salt structures in the context of energy transition. They provide important insights that can help the design of salt caverns for H2/CH4 storage by identifying areas with broadly homogenous halite-rich salt, 2) avoiding drilling through sheared and highly-stressed and strained intra-salt heterogeneities, and 3) constraining minibasin architecture and evolution, improving the understanding of the distribution and geometry of CO2 reservoirs.

How to cite: Pichel, L., Huismans, R., Theunissen, T., Delahaye, S., Pichat, A., Callot, J.-P., and Celini, N.: The role of intra-salt heterogeneity on the internal and external geometry of salt bodies – a numerical modelling approach with applications for geo-storage, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7103, https://doi.org/10.5194/egusphere-egu25-7103, 2025.

EGU25-7356 | ECS | Orals | GD6.1

Exploration and Potential of Geologic Hydrogen Production in the Eastern Snake River Plain, Idaho, USA: A Pathway to Net-Zero Emissions 

Trevor Atkinson, Ghanashyam Neupane, Ayowole Fifo, and Kevin Sylla

A significant component to international energy net-zero emission goals is the exploration, production, and utilization of hydrogen. It is estimated that the International Energy Agency’s goal to reduce emissions will require approximately 550 megatons of hydrogen annually. While traditional generation methods through electrolysis (green hydrogen) and from fossil fuels (blue hydrogen) are potential pathways, they each come with challenges in terms of critical minerals consumption and CO2 sequestration. An alternative and promising source of meeting these goals is geologic hydrogen, naturally produced within the Earth's subsurface. Recent studies estimate that over 20 megatons of hydrogen seep from various geological formations annually. A team led by industry pioneers, Pristine Energy and researchers from the Idaho National Laboratory aim to explore the potential of geologic hydrogen in the Eastern Snake River Plain (ESRP), Idaho, USA. The ESRP is characterized by iron-rich basalt formations and mid-crustal mafic sills, both conducive to hydrogen production through serpentinization. Additionally, geothermal gradients and geochemical fingerprinting suggest the potential for rapid serpentinization at depth, giving insight into geologic hydrogen conversion kinetics. This project will proceed through a systematic approach including a thorough literature review, detailed field sampling, field instrumentation and measurements, lab characterization, and preliminary modeling. Gas, water, and soil samples will be collected from identified fissures, faults, hot springs, and existing wells to identify source and estimate rates and quantities of generated hydrogen. Hydrogen concentrations will be measured using advanced sensors and characterized via gas chromatography-mass spectrometry (GC-MS). High-seepage locations will undergo continuous monitoring to understand seasonal variations in hydrogen emissions. This innovative approach leverages the unique geological attributes of the ESRP to contribute significantly to geologic hydrogen exploration and assessment workflows, and ultimately to the global hydrogen supply, supporting net-zero emission goals.

How to cite: Atkinson, T., Neupane, G., Fifo, A., and Sylla, K.: Exploration and Potential of Geologic Hydrogen Production in the Eastern Snake River Plain, Idaho, USA: A Pathway to Net-Zero Emissions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7356, https://doi.org/10.5194/egusphere-egu25-7356, 2025.

EGU25-7428 | Orals | GD6.1

Deformation controlled fluid mass-transfer processes in ancient orogens  

Graham Hill, Ben Friemann, Eric Roots, Phil Wannamaker, Virginia Maris, Rasmus Haugaard, Jochen Kamm, Svetlana Kovacikova, Radek Klanica, Andy Calvert, Jim Craven, and Richard Smith

Despite abundant empirical evidence, the details of coupled deformation and mass transfer processes within a framework of the crustal architecture of ancient orogens remains enigmatic. Geophysical imaging of the Larder Lake-Cadillac deformation zone, a well-endowed crustal-scale fault system in the Superior Province of the Canadian Shield, characterises the crustal architecture and fault geometry of the system through the lower crust. By comparing the geophysically determined structure of the Larder Lake-Cadillac deformation zone to stress changes induced by Archean (peak orogeny) rupture of the fault system, we show domains of earthquake-triggered deformation coincide with the geophysically imaged low resistivity zones. These low resistivity zones likely formed due to mineral bearing fluid migration from underlying fertile source zones to downstream (shallower) crustal reservoirs and, ultimately, near surface traps. The multi-disciplinary approach identifies the syntectonic mass-transfer processes and fluid pathways, providing an interpretive framework for unraveling the geophysical manifestation of the deformation controlled processes responsible for upflow of metalliferous fluids that may result in ore deposit formation in collisional orogens. 

How to cite: Hill, G., Friemann, B., Roots, E., Wannamaker, P., Maris, V., Haugaard, R., Kamm, J., Kovacikova, S., Klanica, R., Calvert, A., Craven, J., and Smith, R.: Deformation controlled fluid mass-transfer processes in ancient orogens , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7428, https://doi.org/10.5194/egusphere-egu25-7428, 2025.

EGU25-8201 | ECS | Posters on site | GD6.1

Influence of Intra-Salt Lithological Variability on Salt Tectonics: A numerical modelling approach 

Manel Ramos, Ritske Huismans, Leonardo Muniz Pichel, Thomas Theunissen, Jean-Paul Callot, Alexandre Pichat, Naim Célini, Sabine Delahaye, and Claude Gout

Understanding the internal structure of intra-salt layers within deformed salt bodies is crucial for geo-energy storage in salt-bearing basins. This study integrates high-resolution 2D finite element numerical modelling to explore how variations in salt stratigraphy, lithological heterogeneity, and post-salt sedimentation patterns influence deformation processes and the internal architecture of diapiric salt structures across different basin geometries. Specifically, we examine the impact of lithological variability by systematically varying the position and thickness of frictional-plastic, relatively strong intra-salt layers (e.g., anhydrite or carbonates) within a viscous layered salt sequence. The position of the strong intra-salt layer within a salt body significantly influences salt flow dynamics, internal and external diapir morphology, and overburden deformation. When located at the top, the strong layer acts as a stiff cap, restricting upward salt flow and producing broader diapirs with limited overburden deformation. When located in the middle, it localizes strain within the salt, leading to sharper and more discrete diapirs. When located at the bottom, it enhances upward salt flow of the overlying weak salt layer, resulting in tall, narrow, and more intrusive diapirs with more pronounced overburden deformation. In all cases, the strong intra-salt layer breaks and forms boudins, which vary in dimensions, distribution and structural complexity according to their different position and thickness. These intra-salt boudins can be transported by the salt flow to the upper parts of salt structures, but are often trapped at diapir pedestals, beneath diapir flanks, or under minibasins, where they experience repeated folding and refolding as the weaker, less dense salt flows around them. The presence of this heterogeneous intra-salt layer alters the flow paths of the weaker salt and controls both the geometry of salt structures and associated deformation in the overburden. These findings underscore the critical role of stratigraphic and tectonic controls in shaping both the external and internal architecture of salt diapirs, patterns that are particularly relevant for the North Sea, where salt structures play a crucial role in emerging geo-energy storage.

How to cite: Ramos, M., Huismans, R., Muniz Pichel, L., Theunissen, T., Callot, J.-P., Pichat, A., Célini, N., Delahaye, S., and Gout, C.: Influence of Intra-Salt Lithological Variability on Salt Tectonics: A numerical modelling approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8201, https://doi.org/10.5194/egusphere-egu25-8201, 2025.

EGU25-8374 | ECS | Posters on site | GD6.1

Exploration of “fairy circles” associated with natural hydrogen seepages with synthetic aperture radar interferometry and backscatter analysis 

Eszter Békési, Csilla Szárnya, Alain Prinzhofer, Anna Twaróg, Kristóf Porkoláb, and Gábor Tari

With the increasing demand for alternative energy sources, natural hydrogen is gaining attention for commercial exploitation. Naturally accumulated hydrogen is only utilized today at the field of Bourakébougou, Mali, highlighting major knowledge gaps in the behaviour of hydrogen systems and in the related exploration-production workflows. Circular depressions called “fairy circles” represent a surface manifestation of hydrogen seeps that commonly occur in continental cratons and are formed relatively quickly (few years). Apart from the topographic imprint of these ~100 m to 2 km diameter depressions, a major signature of the structures is a vegetation anomaly; characterized by a zone of dying vegetation inside the circle, and a ring of healthy, enriched vegetation in their surroundings. Although the connection of surface H2 seeps to deep-seated H2 sources has been implied in several case studies, the exact mechanism of fairy circle formation is still largely unknown, together with the underlying generation, migration, and accumulation processes of H2.

Satellite images are widely used for the mapping of fairy circles, but these observations are mainly restricted to passive satellite sensors without monitoring any temporal changes of the structures. In this study we used Synthetic Aperture Radar (SAR) images acquired by the European Space Agency’s Sentinel-1 satellites to monitor the evolution of fairy circles in terms of morphological and vegetational changes in two demonstration areas: in the Sao Francisco Basin of Brazil, and in the Lublin Basin of SE Poland. In both cases, the duration of the monitoring was ~5 years, with a temporal resolution of ~1 month. We applied the Interferometric Synthetic Aperture Radar (InSAR) method to map ground motions associated with the potentially active surface deformation of fairy circles. We extended the ground motion time series with SAR backscatter analysis to identify changes in the strength of the backscattered signal through time. The aim of the backscatter analysis was to identify any rapid changes associated with the loss/increase of vegetation linked to H2 degassing. Results show significant ground motion and vegetation anomalies associated with fairy circles in the Sao Francisco Basin (Brazil). Results are not that evident in the Polish area, mostly due to its poorer suitability for InSAR and backscatter analysis (generally lower coherence areas and presence of agricultural and other artificial activities overprinting natural variations). The SAR-based observations were compared with geochemical measurements for monitoring H2 emissions in the soil in both areas, to better understand the potential link between H2 degassing and morphological and/or vegetation changes. The detailed understanding of subsurface processes responsible for the detected anomalies and H2 seeping cannot be inferred, but important constraints on fairy circle formation are achieved. This study demonstrates the applicability and limitations of InSAR and backscatter analysis for the mapping of actively changing fairy circles over two different areas, with important implications of the methodology for further case studies worldwide and constraints on natural hydrogen systems in general.

How to cite: Békési, E., Szárnya, C., Prinzhofer, A., Twaróg, A., Porkoláb, K., and Tari, G.: Exploration of “fairy circles” associated with natural hydrogen seepages with synthetic aperture radar interferometry and backscatter analysis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8374, https://doi.org/10.5194/egusphere-egu25-8374, 2025.

EGU25-8635 | ECS | Posters on site | GD6.1

Investigating Craton Dynamics and Ore Deposit Formation  

Arijit Chakraborty, Jeroen van Hunen, Andrew Valentine, and Poulami Roy

The concentration of critical minerals and metals occurs within 200 km of the transition between thick and thin lithosphere or cratonic edges1. These cratons are regions comprising thicker lithosphere, which has remained stable for billions of years. The critical minerals are initially sourced from the mantle by a range of deep Earth geophysical, geochemical, and tectonic processes, to be further concentrated near the Earth’s surface via hydrothermal processes. These deep Earth processes involving mantle melting also play a crucial role in cratonic stability, and therefore, the improved understanding of these will help unravel intricate connections between craton dynamics and ore deposit formations. 

 The formation and evolution of cratons play a crucial role in the development of those critical minerals. Cratons formed under different scenarios have different internal structures, which, in turn, influence subsequent tectonics and melting scenarios. One of the challenges is how to deal with the vastly different time and length scales in these processes (e.g. between mantle dynamics and melt processes). Preliminary results regarding the best way to capture the processes of craton formation and stability under different geologic scenarios using numerical models developed with the ASPECT geodynamical software tool (REF) will be presented. 

References: 

  • Hoggard, Mark J., Karol Czarnota, Fred D. Richards, David L. Huston, A. Lynton Jaques, and Sia Ghelichkhan. “Global Distribution of Sediment-Hosted Metals Controlled by Craton Edge Stability.” Nature Geoscience 13, no. 7 (July 2020):504–10.https://doi.org/10.1038/s41561-020-0593-2 

How to cite: Chakraborty, A., van Hunen, J., Valentine, A., and Roy, P.: Investigating Craton Dynamics and Ore Deposit Formation , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8635, https://doi.org/10.5194/egusphere-egu25-8635, 2025.

EGU25-8941 | ECS | Posters on site | GD6.1

Geological characterization of the Tertiary Piedmont Basin geothermal system: new insights from structural and stratigraphic analyses  

Maria Isabel Vidal Reyes, Simone Reguzzi, Mattia Marini, Aurora Petagine, Niccolo Menegoni, Chiara Amadori, Matteo Maino, Magdala Tesauro, and Fadi H. Nader

The Tertiary Piedmont Basin (TPB) in northwest Italy is a wedge-top basin developed during Eocene—Pliocene times in the Alps-Apennines tectonic junction. It accommodates, on average, 3 km of clastic sedimentary units with significant lateral facies variations, and several basin-scale unconformities tectonically-controlled. The basin experienced deformation under markedly different tectonic regimes, developing long-lived kilometric structures that affected both the sedimentary successions, and the underlying metamorphic rocks of the Ligurian Alps. The presence of several thermal springs, relatively high surface heat-flow, and locally high geothermal gradient in the TPB, suggests a deep groundwater circulation and heating most likely in a reservoir hosted within the Alpine metamorphic rocks, i.e., the basement.

The geothermal system of the basin is not fully understood, since it still lacks a comprehensive and detailed geological/geophysical model of the basin-basement present-day structure. Aiming to fulfill this gap, this study shows structural analyses performed in the TPB and its Alpine basement at different scales through field-based characterizations, Digital Outcrop Model-based fracture mapping, and seismic interpretation. The integration of these structural results coupled with the spatial distribution of the basement and overlying sedimentary cover, enables a preliminary evaluation of potential reservoir or seal units in the geothermal system. These outcomes provide an adequate conceptual model to better understand the geothermal systems of the TPB, and other systems in analogue settings, having geodynamic peculiarities like slab switches or brake-off.

How to cite: Vidal Reyes, M. I., Reguzzi, S., Marini, M., Petagine, A., Menegoni, N., Amadori, C., Maino, M., Tesauro, M., and Nader, F. H.: Geological characterization of the Tertiary Piedmont Basin geothermal system: new insights from structural and stratigraphic analyses , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8941, https://doi.org/10.5194/egusphere-egu25-8941, 2025.

EGU25-9147 | Posters on site | GD6.1

Thermal state of La Palma (Canary Islands) from a data-integrative approach 

Ivone Jimenez-Munt, Angela Maria Gomez-Garcia, Mauro Cacace, Magdalena Scheck-Wenderoth, Judith Bott, Ana Maria Negredo, Juanjo Ledo, Fatima Martin-Hernández, and Aliss Bejerano

The Canary Islands stand out as a prime region within Spanish territory with significant potential for harnessing high enthalpy geothermal resources due to their active volcanic activity. La Palma, one of the youngest islands in the archipelago, has witnessed at least seven volcanic eruptions over the past 500 years, with the most recent one occurring in 2021. Despite these compelling signs, the development of high enthalpy geothermal power plants has not been pursued on the island, mainly because of the financial risk involved in such project and the lack of detailed geophysical data that can support the correct characterization of the geothermal potential on the island. Accordingly, a data-integrative approach that aids the characterization of potential geothermal sites will reduce such uncertainties, supporting the drilling planning phase of the project. Since the last eruption in 2021, several new geophysical experiments and projects have been undertaken within La Palma Island, aiming to understand the present-day configuration of the subsurface. In this study, we integrate the newly geophysical data in order to build a 3D thermal model that is consistent with the geological structure of the island. This research is funded by the Spanish Government projects PRX23/00106 and PID2022-139943NB-I00

How to cite: Jimenez-Munt, I., Gomez-Garcia, A. M., Cacace, M., Scheck-Wenderoth, M., Bott, J., Negredo, A. M., Ledo, J., Martin-Hernández, F., and Bejerano, A.: Thermal state of La Palma (Canary Islands) from a data-integrative approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9147, https://doi.org/10.5194/egusphere-egu25-9147, 2025.

EGU25-9976 | ECS | Posters on site | GD6.1

A new model for the thickness and thermal structure of the African lithosphere: implications for the distributions of kimberlites, carbonatites and critical mineral deposits 

Siyuan Sui, Yihe Xu, Sergei Lebedev, Emilie Bowman, Javier Fullea, and Sally Gibson

The structure, thickness, lateral heterogeneity, and temporal evolution of the lithosphere significantly influence the distribution of kimberlites, carbonatites, and sediment-hosted mineral deposits, including rare earth elements (REE) and critical metals (e.g., Nb and Ti) that are essential for advancing the transition to green energy.

Seismic data provide critical information on the thermal structure of the lithosphere and underlying mantle. However, seismic tomographic models are inherently non-unique. This can be remedied, to a large extent, by thermodynamic inversions, which utilize computational petrology and offer an effective approach to connecting seismic observations to the thermal structure of the lithosphere and mantle.

We present a new model of the African lithosphere’s thickness and thermal structure, derived from state-of-the-art sampling with seismic surface wave data. The model incorporates both Rayleigh and Love waves, to account and correct for seismic anisotropy of the elastic properties. Rayleigh and Love wave data in the 20–300 s range are inverted, on 1°×1° grids, for the upper-mantle temperature and lithospheric thickness, from which upper-mantle density and seismic velocities are calculated, with attenuation corrections. Radial anisotropy, seismic velocities in the crust, transition zone and uppermost lower mantle, and crustal density are also inversion parameters, the latter constrained primarily by the surface elevation. The resulting model reveals distinct regional variations in the lithospheric thickness that reveal deep lithospheric expressions of known crustal geology. Thick lithosphere (>220 km) is found beneath large parts of the West African Craton, Congo Craton, and Zimbabwe Craton. Thin lithosphere (<70 km) is predominantly observed along the East African Rift.

We analyse the new lithosphere model jointly with recent datasets of the distribution of different types of igneous rocks across the continent. These include kimberlites, which were emplaced at locations with thick cratonic lithosphere; basalts, which are emplaced at locations with thin lithosphere; and carbonatites that are commonly found on intermediate-thickness lithosphere (Gibson et al. 2024). Statistics analysis of the locations of these rock samples shows that kimberlites mostly are found within cratons, with some notable exceptions. Most Neogene basalts are in the East African Rift Zone, with a 50–100 km lithosphere. Carbonatite complexes and their associated REE deposits, are typically observed in clusters in the transition regions from cratonic to non-cratonic lithosphere.

This new lithospheric thickness and temperature model enhances our understanding of the dynamics and evolution of the African lithosphere. Furthermore, it provides valuable insights into the processes that govern the generation and spatial distribution of rocks of different types and the associated primary critical mineral deposits.

 

Gibson, S., McKenzie, D. & Lebedev, S. (2024). The distribution and generation of carbonatites. Geology 52, 667–671.

How to cite: Sui, S., Xu, Y., Lebedev, S., Bowman, E., Fullea, J., and Gibson, S.: A new model for the thickness and thermal structure of the African lithosphere: implications for the distributions of kimberlites, carbonatites and critical mineral deposits, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9976, https://doi.org/10.5194/egusphere-egu25-9976, 2025.

EGU25-10051 | Posters on site | GD6.1

Stress, pore pressure, sediment compaction, deformation, temperature and fluid flow in the SE German part of the North Alpine Foreland Basin 

Michael Drews, Florian Duschl, Saeed Mahmoodpour, Enzo Aconcha, Julian Breitsameter, Peter Obermeier, Indira Shatyrbayeva, Parisa Babaie, Christian Tomsu, and Florian Einsiedl

The North Alpine Foreland Basin is the peripheral foredeep of the Northern Alps, extending from Lake Geneva in the West to Upper Austria in the East. The largest portion of the foredeep consists of an undeformed part, called Foreland Molasse, and a small, deformed belt along the North Alpine Thrust Front, called Subalpine Molasse. Spanning up to 150 km in N-S direction, the North Alpine Foreland Basin has its widest extent in SE Germany (Bavaria). Here, the physical properties of the Cenozoic basin fill and its underlying Mesozoic passive margin sediments display a high degree of heterogeneity in both the Foreland Molasse and Subalpine Molasse parts. Since 2016, we systematically analysed data from more than 300 deep wellbores, with vertical depths up to 5 km below ground level, to understand the distribution and interplay of these heterogeneities: We used minimum stress magnitude measurements such as formation integrity and leak-off tests in combination with geophysical borehole measurements such as density and velocity to infer the distribution of lateral and vertical stresses in the SE German part of the North Alpine Foreland Basin. Collection of pore pressure indicators and measurements such as drilling mud weights, drilling problems, well tests and wireline formation tests and their correlation with vertical stress and sediment compaction allowed us to also infer the regional distribution of pore pressure and to model the variable styles of deformation of the Subalpine Molasse along the North Alpine Thrust Front. In this contribution, we give a graphical overview of how stress, pore pressure and deformation are linked and driven by sediment composition and compaction. We also set our findings into context with high frequency, large amplitude variations of temperature and fluid flow patterns, proposing an updated model for the distribution and interference of physical properties and processes in the North Alpine Foreland Basin in SE Germany.

How to cite: Drews, M., Duschl, F., Mahmoodpour, S., Aconcha, E., Breitsameter, J., Obermeier, P., Shatyrbayeva, I., Babaie, P., Tomsu, C., and Einsiedl, F.: Stress, pore pressure, sediment compaction, deformation, temperature and fluid flow in the SE German part of the North Alpine Foreland Basin, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10051, https://doi.org/10.5194/egusphere-egu25-10051, 2025.

EGU25-10415 | Orals | GD6.1

Serpentinization-sourced hydrogen systems in rift inversion orogens: a geological/holistic perspective 

Gianreto Manatschal, Marc Ulrich, Pauline Chenin, Francesca Dimasi, Quentin Gasser, Eric C. Gaucher, Emmanuel Masini, Cuimei Zhang, Peter Alt-Epping, Frank Zwaan, and Nick Kusznir

Serpentinization-sourced H2 has become a promising source of decarbonated energy. It can be generated in fiver tectonic settings, namely: (1) intra-craton settings, (2) divergent settings such as hyperextended rifts, ocean continent transitions and mid ocean ridges, (3) subduction systems, (4) obduction, and (5) rift-inverted orogens. Most recently, many studies have been focusing on parts of the H2-system, i.e., the kitchen, plumbing system, reservoir, cap rock and trapping and preservation mechanisms or on the detection of leaking natural H2 systems at or near the surface. However, a holistic understanding of a serpentinization-sourced H2 system is still in its infancy and an exploration protocol tailored to the different tectonic settings is missing to date.   

In our study, we aim to develop a protocol to predict, quantify and explore serpentinization-sourced H2 systems in rift-inverted orogens. To do so, we use the Grisons area (SE Alps in Switzerland) as a field analogue. In this area all play-elements of the serpentinization-sourced H2 system exist and can be accessed and the rift and convergent structures are well exposed and investigated. This allows us to examine the interplay, in time and space, between the play-elements of a serpentinization-sourced H2 system and to develop a predictive exploration protocol. In this perspective, we first seek  to define a serpentinization-sourced H2 system in a rift-inversion orogen and second to address when and where the serpentinization-sourced H2 forms, what are the essential play-elements and how they interact in time and space, impacting the location and timing of H2 production by considering the two dominant parameters, temperature and access to water, which determine entry into the serpentinization window (kitchen) for mantle rocks. In our presentation, we show the first preliminary results of our holistic, geological approach aiming to integrate different data sets from the Grisons area. We are aware that to develop a predictive play-element based exploration protocol for a serpentinization-sourced H2 system in rift-inverted orogens, similar to that developed in oil and gas systems, further studies will be necessary.

How to cite: Manatschal, G., Ulrich, M., Chenin, P., Dimasi, F., Gasser, Q., Gaucher, E. C., Masini, E., Zhang, C., Alt-Epping, P., Zwaan, F., and Kusznir, N.: Serpentinization-sourced hydrogen systems in rift inversion orogens: a geological/holistic perspective, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10415, https://doi.org/10.5194/egusphere-egu25-10415, 2025.

EGU25-10972 | ECS | Orals | GD6.1

Fault-hosted hot springs of the Rhône Valley in the context of varying regional-scale neotectonics 

Timothy Schmid, Marco Herwegh, Alfons Berger, Tobias Diehl, Herfried Madritsch, Daniela van den Heuvel, Christoph Wanner, and Larryn Diamond

Orogenic geothermal systems develop when meteoric water infiltrates the subsurface at high elevations, heats up along a deep circulation path due to the background geothermal gradient and eventually emerges at the surface in low topographic sites as localized hot springs. Such systems depend on permeable fault geometries; however, in orogenic settings fluid-discharge zones may additionally be controlled by the configuration of topography, nappe geometry, fault patterns and unconsolidated deposits that can conceal the bedrock structure. Hence, it is crucial to study local hot springs in the context of fault structures related to regional tectonics in order to predict the locations of blind geothermal systems. The Rhône Valley is a favourable site for such a study, as it shows the highest seismic activity in Switzerland and hosts several clusters of hot springs aligned along the regional Rhône-Simplon fault system.

Here, we combine data sets on geodynamics such as geodesy of recent crustal movements, regional recent stress fields, relocated hypocenters and focal mechanisms as well as structural field data to interpret the hot spring occurrences in the context of regional geodynamics. Our data suggest the presence of three adjacent structural domains: (1) A domain on the NW flank of the Rhône fault characterized by a NW–SE oriented maximum principal stress, high seismicity, and a pervasive network of strike- slip dominated faults; (2) a zone encompassing the Rhône Valley floor with transtensive, dilatant zones along strike-slip fault segments; and (3) a zone on the southern flank of the valley floor subjected to a recent NE–SW extension expressed by dominantly normal to transtensional faulting focal mechanisms. This southern domain constitutes the SW-extruding hanging wall block of the Simplon low-angle normal fault. The block is bounded by two crustal scale strike-slip faults, the dextral Rhône strike-slip fault in the NW and the sinistral Ospizio Sottile line in the SE.

In summary, our study highlights the importance of the large-scale tectonic setting for understanding and exploring fault controlled and hence, strongly localized geothermal resources in orogenic settings.

How to cite: Schmid, T., Herwegh, M., Berger, A., Diehl, T., Madritsch, H., van den Heuvel, D., Wanner, C., and Diamond, L.: Fault-hosted hot springs of the Rhône Valley in the context of varying regional-scale neotectonics, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10972, https://doi.org/10.5194/egusphere-egu25-10972, 2025.

EGU25-11375 | Orals | GD6.1

Iron redox state of serpentinized mantle rocks through a Wilson cycle: implications for serpentinization-sourced hydrogen systems 

Francesca Dimasi, Marc Ulrich, Manuel Muñoz, Flora Hochscheid, and Gianreto Manatschal

Climate-CO2 emission models point to the urgency for European society to transition from high to low carbon energy sources. In this frame, H2 could be a key component of the decarbonization strategy. Among the various colours of H2, white (i.e., native) H2 is one of the most promising. The most efficient way to produce native H2 is serpentinization, a high temperature hydrothermal process that forms serpentinites from Earth mantle rocks. This hydrothermal alteration transforms primary magmatic Fe-Mg-bearing silicates (olivine, pyroxenes) into secondary hydrous minerals (e.g. serpentine, brucite) and oxides (magnetite). Serpentinization also produces molecular hydrogen (H2) through oxidation of ferrous Fe (FeII) released from the dissolving primary minerals, to ferric Fe (FeIII) that precipitates in serpentine and magnetite. The serpentinization process has been extensively documented at various geological settings such as mid-ocean ridges or subduction zones. In contrast, it has received much less attention at rift inverted orogens and continental rifts, representing classical sources of oil and gas, but nowadays being at the forefront of carbon capture, geothermal energy, and new decarbonated energy resources such as native hydrogen. In conclusion, understanding the iron redox state in a Wilson cycle will allow us to predict when, where and how serpentinized sourced hydrogen is produced, which is a prerequisite to develop a successful exploration strategy.

Our approach to achieve this goal is based on a representative sampling area, state-of-the-art analyses and modelling (the evolution of redox and the production of H2). A series of analytical methods will be conducted on serpentinites from well-defined sites (Tasna, Platta, Totalp, Val Malenco and Lanzo) documenting the Wilson cycle of the Alpine-Tethys system. The analysis will constrain the conditions  of serpentinization, i.e., temperature of fluid-rock interactions, PT paths recorded by mantle rocks, and redox state. Finally, the new data will constrain the evolution of iron speciation and H2 production during serpentinization and may be used to either test or calibrate numerical modelling results used for the quantification of H2 production.

How to cite: Dimasi, F., Ulrich, M., Muñoz, M., Hochscheid, F., and Manatschal, G.: Iron redox state of serpentinized mantle rocks through a Wilson cycle: implications for serpentinization-sourced hydrogen systems, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11375, https://doi.org/10.5194/egusphere-egu25-11375, 2025.

EGU25-11413 | Posters on site | GD6.1

Petrological and geophysical characterization of a paleo natural hydrogen kitchen – serpentinites of the Münchberg Massif, Germany 

Peter Klitzke, Meike Bagge, Maximiian Hasch, Nikola Koglin, Antonia Ruppel, Hamed Fazlikhani, Felix Johann, Jan-Felix Goldmann, Alexander Löwer, and Christian Ostertag-Henning

One of the main challenges in studying a natural hydrogen system is that ultramafic rocks - potential source rock for hydrogen generation by serpentinization - are often buried deep within the subsurface. The serpentinites of the metamorphic Münchberg Massif, obducted during the Variscian orogeny in Devonian times, offer a unique window into deep crustal and upper mantle processes. As part of an integrated study, we have acquired airborne magnetic and strapdown gravity data, seismic reflection profiles, as well as detailed petrological and geochemical analysis. This approach enables a multi-scale interpretation of the tectonic evolution, serpentinization processes, and associated fluid-rock interactions, mineralogical transformations, and implications for paleo-natural hydrogen generation in the Münchberg Massif. 

Serpentinite rock bodies are exposed at multiple outcrops across the Münchberg Massif. Geochemical analyses of major and rare earth elements indicate that serpentinites from both the Peterleinstein (west) and the Zell region (south) share a similar protolith of harzburgitic composition. However, different serpentine minerals dominate at the different locations. The Zell serpentinites, predominantly antigorite, appear to have undergone serpentinization at greater depths and higher temperatures than the Peterleinstein serpentinites, which are dominated by lizardite. Conversely, Peterleinstein demonstrates a higher degree of serpentinization, likely indicating increased fluid availability during the process. The sequence of events during serpentinization is evident in spatially resolved analyses of different generations of serpentine minerals in thin sections using microscopic and Raman micro-spectroscopic analyses.

Initial interpretation of the airborne magnetic data reveals a series of positive high-frequency anomalies with amplitudes of up to ~160 nT, associated with magnetite enrichment, a by-product of serpentinization and hydrogen generation across the Münchberg Massif. Petrological analyses confirm the presence of magnetite-bearing serpentinites. However, preliminary on-site magnetic susceptibility measurements do not resolve differences in the degree of serpentinization. Combined petrophysical, seismic, gravity and magnetic interpretation and modeling will constrain the extent of serpentinization in the subsurface and evaluate the role of major faults as fluid conduits during serpentinization.

How to cite: Klitzke, P., Bagge, M., Hasch, M., Koglin, N., Ruppel, A., Fazlikhani, H., Johann, F., Goldmann, J.-F., Löwer, A., and Ostertag-Henning, C.: Petrological and geophysical characterization of a paleo natural hydrogen kitchen – serpentinites of the Münchberg Massif, Germany, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11413, https://doi.org/10.5194/egusphere-egu25-11413, 2025.

EGU25-11735 | ECS | Orals | GD6.1

Artificial Smoker: Geophysical characterization of an ultraslow ridge system for sustainable resource management 

Bhargav Boddupalli, Børge Arntsen, Tim Minshull, Ketil Hokstad, Sylvie Leroy, Ståle Johansen, Louise Watremez, Ana Corbalan, and Lars Sørum

Hydrothermal circulation is a fundamental Earth process that transfers elements and minerals from the crust and mantle to the oceans. This circulation commonly occurs along tectonic plate boundaries in the oceans, where heat sources are located at relatively shallow depths (~2–3 km). Cold seawater percolates downward, becomes heated, and is enriched with minerals from the host rock and magmatic volatiles. The resulting hot fluids (exceeding 300°C) rise buoyantly and are expelled into the ocean through chimney-like structures on the seafloor, commonly referred to as "Black Smokers." The ejected particles settle on the seafloor, forming rich mineral deposits known as "Seafloor Massive Sulfide" (SMS) deposits, making mid-ocean ridges highly attractive for meeting future mineral demands. Moreover, ridge settings hold significant potential for geothermal energy, white hydrogen production, and other valuable resources. However, harnessing these resources requires a thorough understanding of the complex hydrothermal systems to develop sustainable resource management strategies.

Hydrothermal venting sites are widespread along the mid-ocean ridge system, occurring at all spreading rates and across diverse geological settings. However, the mechanisms driving hydrothermal processes vary depending on factors such as the presence of magma bodies, permeable zones, tectonic activity, and temperature. At ultraslow spreading ridges, where spreading rates are less than 20 mm/yr—such as the Southwest Indian Ridge, Mohns Ridge, and Knipovich Ridge—tectonic processes dominate over magmatic activity, resulting in the exhumation of ultramafic material to the seafloor along large-scale detachment faults.

In this study, we developed two-dimensional, high-resolution velocity models through the crust and uppermost mantle of the Southwest Indian Ridge using wide-angle ocean-bottom seismic data. We present two ~150 km-long, high-resolution P-wave velocity models orthogonal to each other, running across and along the ridge axis at 64°30’E. We employed a state-of-the-art imaging technique known as full waveform inversion (FWI) using data from 32 ocean-bottom seismometers positioned along the two profiles. FWI is a data-fitting method in which the forward operator iteratively predicts the observed data by backpropagating the misfits to update the velocity model, thereby producing higher-resolution images of the subsurface.

Based on our high-resolution velocity models, we observe finer patterns of velocity anomalies compared to traveltime models, revealing more detailed variations in the degree of fluid-rock interaction. These interactions are influenced by the presence of faults and the extent of tectonic damage, aiding in the mapping of hydrothermal circulation. Additionally, our high-resolution images provide an improved understanding of the distribution of serpentinization and its correlation to mode of spreading. Overall, the high-resolution velocity models support the assessment of the feasibility of "Artificial Smoker," which replicates natural smokers, for the environmentally sustainable extraction of minerals, white hydrogen, and geothermal resources.

How to cite: Boddupalli, B., Arntsen, B., Minshull, T., Hokstad, K., Leroy, S., Johansen, S., Watremez, L., Corbalan, A., and Sørum, L.: Artificial Smoker: Geophysical characterization of an ultraslow ridge system for sustainable resource management, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11735, https://doi.org/10.5194/egusphere-egu25-11735, 2025.

EGU25-12600 | ECS | Orals | GD6.1

Isotopic Insights into the Origins of N₂-H₂-CH₄ emanations in the New Caledonia Ophiolite 

Jean de la Paix Izerumugaba, Anne Battani, Eric Deville, Camille Maziere, Julie Jeanpert, Olivier Lhote, Fréderic Mouthereau, Willy Foucher, Olivier Monge, and Anthony Ranchou-Peyruse

Natural emanations consisting of N₂-CH₄-H₂ type gases have been documented across the peridotite nappe of the New Caledonia Ophiolite [1], and the presence of H2 has been attributed to serpentinization [2, 3]. We present new major and noble gas compositional and isotopic data from low to high H2 bubbling gas seep sites from both the south (e.g: Lembi River (≤ 20% H2), Les Pirogues River (≤ 15%), Pourina (≤ 10%)), and north east klippes of the Ophiolite (e.g: Fanama and Nemwegi (≤ 300ppm)), providing new insights into gas origins that can be compared to other serpentinization systems (e.g: Oman, Italy, Turkey, and the Philippines).

Results show that gases are dominated by N2 (60-95%; d15N ranging from -0.2 to +0.1‰ vs air), while the H2 content can reach up to 35% with dD ranging from -740 to -710‰ VSMOW. CH4 reaches up to 20% with d13C ranging from -40‰ to -3.6‰ VPDB. Such major gas composition and isotopic values are characteristic of serpentinization [4, 5]. Additional factors, such as olivine-rich peridotite rocks, precipitation of magnetite, carbonates, and brucite, along with the elevated pH of spring waters (up to 10.5), confirm an active serpentinization system. Hydrogen H2-CH4-H2O isotopic fractionation factors suggest that, despite not being at equilibrium, the hydrogen-bearing fluids are formed at around 50°C, in comparison to 95°C, which was determined using magnetite-dolomite O₂ fractionation [6]. H2 and CH4 likely result from low-temperature serpentinization and processes involving inorganic carbon, respectively; potentially catalysed by Ni, Cr, and Chromitite-hosted Ru [7] which are enriched in the peridotite [1, 8]. Microbial activity indicators such as the presence of biogenic methane, when present, aligns with documented microbial communities.

Helium isotopic data (3He/4He) indicate signatures ranging from predominantly radiogenic (0.3 Ra) in the north, where the crust is thick [2], to ASW-like values in the central south (Lembi and La Coulée), to ~25% mantellic contribution in the southernmost coastal Prony region. We argue that the air-like signature is indicative of the degassing of circulating air-saturated groundwater, which aligns well with interpretations that air-like N₂ present in serpentinization systems may originate from aquifers [2, 3, 4].

Seismic and tectonic data reveal multiple deep faults and fractures in the massif du Sud [9], as well as a shallow Moho and 20 km-deep earthquakes that are indicative of active tectonics detected beneath the Prony area [10]. This explains the facilitated migration of mantle fluids to the surface at Prony.

[1] Maurizot et al., 2020(c). Geol. Soc. Lond. Mem. 51(1), 1–12

[2] Deville and Prinzhofer, 2016. Chem. Geol. 440, 139–147

[3] Monnin et al., 2021. JGR Biogeosci. 126, e2021JG006243.

[4] Vacquand et al., 2018. Geochim. Cosmochim. Acta 223, 437–461.

[5] Etiope, 2017. Procedia Earth Planet. Sci. 17, 9–12.

[6] Corre et al., 2023. Sci. Rep. 13(1), 19413.

[7] Molinet-Chinaglia et al., 2024. ChemCatChem 16(24), e202401213.

[8] Maurizot et al., 2020(f). Geol. Soc. Lond. Mem. 51(1), 247–277.

[9] Lagabrielle et al., 2005. Tectonophysics 403(1–4), 1–28.

[10] https://submap.fr

How to cite: Izerumugaba, J. D. L. P., Battani, A., Deville, E., Maziere, C., Jeanpert, J., Lhote, O., Mouthereau, F., Foucher, W., Monge, O., and Ranchou-Peyruse, A.: Isotopic Insights into the Origins of N₂-H₂-CH₄ emanations in the New Caledonia Ophiolite, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12600, https://doi.org/10.5194/egusphere-egu25-12600, 2025.

EGU25-12845 | Orals | GD6.1

Fault-controlled groundwater recharge from Alpine units into Upper Jurassic Limestone of the North Alpine Foreland Basin (SE Germany) 

Florian Duschl, Enzo Aconcha, Regina Ettenhuber, Christian Tomsu, Florian Einsiedl, and Michael Drews

Fluid temperatures in the Cenozoic basin fill of the North Alpine Foreland Basin (SE Germany) are locally significantly lower compared to adjacent areas of the basin. In the greater Rosenheim area, formation temperatures at a depth of 4000 mbs range ca. 80 K lower than expected with respect to a typical regional geothermal gradient of 28-30 K/km. Possible explanations for this so-called Wasserburg Trough anomaly include thermal blanketing by rapid deposition of cold sediments, effects of convective and advective heat transfer in Cenozoic sediments, long-term effects of glacial thermal overprint, increased gravity-driven recharge due to karstification in the underlying Upper Jurassic Limestone, and heat transfer towards the Tauern Window due to a thermal chimney effect. Recent studies on formation fluid ages in the Upper Jurassic Limestone, a prolific, hydrostatically pressured geothermal aquifer, show comparatively young fluid ages of <20 ka which points at local freshwater infiltration at greater depth. Freshwater influx may reduce heat flow, act as a conductive heat barrier and favour karstification. However, fluid overpressure in shales of the Cenozoic overburden does not allow for direct vertical fluid infiltration across the stratigraphic column.

We propose a tectonic control mechanism responsible for freshwater infiltration with the Bavarian Inntal Fault Zone, a normal fault system that was formed during indentation of the Southern Alps in Oligo-Miocene times, acting as a conduit fault. This fault zone is indicated by a steepening of W-E striking fold axes towards the Bavarian Inntal, and the existence of several, valley-parallel sets of NNW-SSE striking normal faults proving WSW-ENE directed extension. Total vertical displacement inferred from cross-sections and field data yield at ≥250 m which is probably sufficient to ensure hydraulic contact between sedimentary strata of the Alpine nappes and underlying Upper Jurassic Limestone in the deeper subsurface. Thereby, freshwater from the Alps could bypass the overpressure zone in the Bavarian Inntal and infiltrate into the Upper Jurassic Limestone aquifer of the foreland basin.

How to cite: Duschl, F., Aconcha, E., Ettenhuber, R., Tomsu, C., Einsiedl, F., and Drews, M.: Fault-controlled groundwater recharge from Alpine units into Upper Jurassic Limestone of the North Alpine Foreland Basin (SE Germany), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12845, https://doi.org/10.5194/egusphere-egu25-12845, 2025.

EGU25-13046 | ECS | Orals | GD6.1

Resolving Whole-Lithospheric Architecture for Mineral Prospectivity and Beyond: A Probabilistic Inversion Approach 

Riddhi Dave, Andrew Schaeffer, Fiona Darbyshire, and Juan Carlos Afonso

The architecture of the lithosphere is shaped by diverse geodynamic processes, including the presence of metasomatized mantle volumes, lithospheric thickness transitions, crustal- and mantle-scale fluid migration pathways, and the influence of plumes and subducting slabs. These features are preserved in the physical and chemical structures of the lithospheric mantle and sub-lithospheric upper mantle, providing critical insights into mineral systems and resource prospectivity.

To address these complexities within the Canadian lithosphere and mantle, we apply a probabilistic inversion framework, LitMod, which integrates geological constraints with multiple geophysical techniques and incorporates a priori geochemical information. This unified approach enables the resolution of key lithospheric features, distinguishing between compositional (e.g., metasomatism) and thermal anomalies.

We present results from the first application of LitMod to Canada, highlighting its capability to map essential geophysical structures and surfaces. Validation of the model’s predictions using independent geochemical datasets underscores the robustness and reliability of our results. Beyond advancing mineral prospectivity, this work contributes to broader geoscientific applications, including refining Glacial Isostatic Adjustment (GIA) models, improving Carbon Capture, Utilization, and Storage (CCUS) strategies, and enhancing seismic hazard assessments.

How to cite: Dave, R., Schaeffer, A., Darbyshire, F., and Afonso, J. C.: Resolving Whole-Lithospheric Architecture for Mineral Prospectivity and Beyond: A Probabilistic Inversion Approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13046, https://doi.org/10.5194/egusphere-egu25-13046, 2025.

EGU25-14781 | ECS | Posters on site | GD6.1

Geodynamic Heterogeneity in Back Arc Basins: Implications for Heat Flow Distribution and Geothermal Energy Potential. 

Abdul-Nazaa Nuhu, Alessandro Decarlis, Andrea Ceriani, and Philip Ball

Using the geodynamic model of Hasterock et al., (2022), Ball et al., (2025) observed that existing natural hydrothermal systems and associated geothermal power plants are distributed across 12 different geodynamic settings.  We observe based on the Hasterock classification only 18 out of 489 power plants (3.6%) are located within Back Arc Basins (BABs). This may lead to the conclusion that, at a global scale, BABs are not highly prospective. However, a much more detailed observation of the various tectonic settings at specific locations shows some incongruencies in the Hasterock geodynamic classification. For example, key power plants such as Larderello, Italy are in fact located in a BAB setting, not in a Volcanic Arc setting (Ball, 2022). At a local scale it is important to refine global models to account for younger deformation that overprint previous tectonic events.

With Larderello as an analogue, we explore the idea that other BABs could be increasingly perspective for geothermal resources if the geodynamic setting is correctly assessed, and the local tectonics is understood. BABs, are extensional basins, typically formed behind active or inactive volcanic arc on the overriding plates. BABs, are known to be associated with high heat flow, due to the interplay of mantle dynamics, slab processes and crustal extension. In this work, we review the first-order controls on heat flow within the Aegean and Tyrrhenian back arc systems. We point to the comprehension of how factors like rapid localization of thinning in the crust and lithospheric mantle impacts heat flow, coupled with sedimentary cover. In detail, we evaluate the role of accessory parameters, like hydrothermal fluids ascending along faults and fractures, the role of intrusions due to patrial melting in response to rapid thinning in the crust and mantle, localizing high heat flows spots and causing significant thermal heterogeneities.

The dynamic settings of BABs could offer intriguing geothermal opportunities, but their structural, magmatic and hydrological histories need to be better understood. BAB’s like the Tyrrhenian and Aegean may provide exceptional opportunities for power generation. Exploration in this geodynamic setting could benefit by using the exploration triangle, which organizes the geological assessment into a hierarchical sequence of tasks. This play-based approach focusses assessment from the geodynamic setting and can be applied at the geothermal systems, and reservoirs scale. Successful application could greatly assist in identifying future prospects for geothermal development,  successfully exploiting BAB’s for power generation.

How to cite: Nuhu, A.-N., Decarlis, A., Ceriani, A., and Ball, P.: Geodynamic Heterogeneity in Back Arc Basins: Implications for Heat Flow Distribution and Geothermal Energy Potential., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14781, https://doi.org/10.5194/egusphere-egu25-14781, 2025.

EGU25-16399 | ECS | Orals | GD6.1

In-soil hydrogen concentration measurements using MONHyTOR. 

Niko Adjie, Clarisse Bordes, Daniel Brito, Djamel Nasri, Eric Normandin, and Christophe Voisin

Soil gas analysis is among the commonly used methods in the early stages of natural hydrogen exploration. While most punctual [H2] measurements can provide information on spatial variation, observing temporal variation requires long-term monitoring. The University of Pau and Adour Countries developed a hydrogen-monitoring instrument called MONHyTOR. It is a passive instrument capable of acquiring [H2], temperature, and relative humidity data with up to 1-s sampling interval at 1-m depth for up to several months in full autonomy.

Preliminary field data from multiple sites show that (1) an “installation peak” is almost systematically observed after drilling; (2) measured [H2] is nil most of the times; (3) daily oscillations are present in some datasets; (4) small-amplitude isolated peaks are seemingly related to weather events such as storm and heavy rain. These observations raise the question regarding the influence of water saturation and pressure balance in the atmosphere-soil-instrument system. To understand them, experiments are carried out in a controlled environment using airtight container filled with coarse homogeneous sand with a given water saturation level, where hydrogen is introduced via low-pressure (mbar) injections of 5%-95% H2-N2 mixture. The aim of this study is to see how variations in the pressure balance impact [H2] measurements by MONHyTOR.

How to cite: Adjie, N., Bordes, C., Brito, D., Nasri, D., Normandin, E., and Voisin, C.: In-soil hydrogen concentration measurements using MONHyTOR., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16399, https://doi.org/10.5194/egusphere-egu25-16399, 2025.

EGU25-16617 | ECS | Orals | GD6.1

Origins of Helium and Hydrogen in South Australia 

Zak Milner, Jon Gluyas, Ken McCaffrey, Bob Holdsworth, Darren Grocke, Darren Hillegonds, Thomas Renshaw, Chris Ballentine, and Philippa Ascough

Releasing only heat and water vapour when burnt, demand for hydrogen (H₂) is expected to increase eight-fold by 2050, driven by growth sectors such as transportation and industrial energy. Natural or gold H₂ is produced in the lithosphere via water radiolysis in U- and Th-rich Precambrian basement (alongside helium (He)) or serpentinization in mafic-ultramafic rocks. Gas occurrences in South Australia have anomalously high H₂ concentrations of up to 95%. It is, therefore, an excellent geographical focus to further understand the principles of H₂ exploration (source, migration, accumulation, and preservation).
This study reports noble gas isotopes (He to Xe) of gases dissolved in groundwater samples collected from 19 locations across the Yorke Peninsula and Adelaide Superbasin, along with their respective ages from radiocarbon dating. Using helium as a proxy, we provide insights into the source and migration of H₂ in South Australia. Through the use of a novel gas diffusion model (Cheng et al. 2023), we also investigate whether an H₂/He gas phase can be produced, critical for their concentration and formation as accessible resources.

How to cite: Milner, Z., Gluyas, J., McCaffrey, K., Holdsworth, B., Grocke, D., Hillegonds, D., Renshaw, T., Ballentine, C., and Ascough, P.: Origins of Helium and Hydrogen in South Australia, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16617, https://doi.org/10.5194/egusphere-egu25-16617, 2025.

There is a growing interest in natural hydrogen as a potential new source of energy with a negligible carbon-footprint, especially compared to all the other human-made hydrogen species. The white (or gold, natural, geologic or geogenic) and orange (or induced) hydrogen became the focus of intense research during the last decade.

From the energy industry point of view the fundamental question arises about natural hydrogen exploration, i.e. how different is it going to look compared to what we are used to in the hydrocarbon industry? After many decades of negligible consideration given to natural hydrogen as a subsurface target there are many papers and presentations published just in the last few years suggesting that many items in our collective industry and academic toolbox could be readily applied to natural hydrogen exploration. The consensus appears to be that three out four of the main petroleum systems elements the hydrocarbon industry tends to focus on in exploration projects are still going to play pivotal roles (i.e. migration, trapping and sealing) and it is only the generation/charge part which follows very different rules for hydrogen systems.

From an exploration point of view, several play types for natural hydrogen indeed appear to be very similar to what the oil and gas industry is used to. These include cases where there is a functioning trap, due to effective top seals. Numerous examples can be found in pre-salt traps worldwide where hydrogen has been documented for a long time as part of existing natural gas accumulations (e.g. Dnieper-Donets Basin, Ukraine, and Amadeus Basin, Australia). Another, but unusual trapping style has been documented in the first hydrogen field discovery in Mali where the top seal is a set of dolerite dykes. In these cases, one expects finite hydrogen resources to be in place and the exploration approach has indeed some resemblance to that of hydrocarbon prospecting.

Another group of natural hydrogen targets revolve around large mega-seeps (fairy circles) and geometrically smaller, but pronounced fault-controlled seepages to the surface. These hydrogen occurrences seemingly have no traps or seals and, therefore, do not find a proper analogue in oil and gas exploration workflows. Strictly speaking, these are not yet hydrogen plays as there are no commercial discoveries associated with them. The hydrogen fluxing along fault planes requires a fresh look at the exploitation of various fault architectures if shallow drilling would target conductive (or “leaky”) faults at shallow depth. In a more traditional exploration workflow, properly mapping and quantifying hydrogen fluxing along fault planes in shallow depth might be the first critical step before more conventional deeper targets (>1000 m) could be addressed. This set of plays promises that if these seeps really correspond to ongoing charge in a dynamic, truly renewable system in a steady-state process, tapping successfully into them would provide infinite resources via a low-flux hydrogen “farming” process.

It is quite likely that natural hydrogen exploration, if it becomes economically successful at one point, will look much more different than similar to hydrocarbon exploration.

How to cite: Tari, G.: Natural hydrogen exploration: it is quite different from looking for hydrocarbons, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16903, https://doi.org/10.5194/egusphere-egu25-16903, 2025.

EGU25-19413 | Posters on site | GD6.1

Geophysical and Geotechnical offshore studies: pioneering contribution to shape Portugal’s wind farm strategy  

Pedro Brito, Luís Batista, Rúben Borges, Pedro Costa, Marta Neres, João Noiva, Ângela Pereira, Carlos Ribeiro, Marcos Rosa, and Pedro Terrinha

The Instituto Português do Mar e da Atmosfera (IPMA) is undertaking extensive high-resolution geophysical and geotechnical studies over two areas proposed for the development of offshore windfarms in Portugal, surveying an area of circa 2000 km2. Leixões and Figueira da Foz study areas are located off the Portuguese mainland west coast, at depths between 120m and 530m, distant 21nm to 35nm to the coastline.

The aim of this work, being conducted between February 2024 and June 2026, is to provide detailed data on the morphology, geology, geophysics and geotechnical properties of the seafloor to inform offshore wind farm developers towards engineering and financial strategies, therefore providing the basis for launching subsequent auctions for the offshore areas listed in the Portuguese National Maritime Spatial Planning Situation Plan.

An initial exploratory campaign, commissioned to the Portuguese Hydrographic Institute, collected the initial MBES data (bathymetry and backscatter) and surface sediment sampling. Furthermore, in August-September 2024, a geophysical survey took place on board IPMA’s NI Mário Ruivo and retrieved over 2100 km of seismic data, from parametric sub bottom profiler (SBP) and multi-channel ultra-high resolution seismic reflection (UHRS). Preliminary results attest the scientific richness of the dataset already collected as well as the complexity and diversity of the seimostratigraphy present in the surveyed areas.  Seabed morphology, sediment textural features, seismic horizons and geohazards have been identified which allow inference of a preliminary geomodel of the areas and the planning of subsequent surveys.

Between May and November 2025 a survey will take place expanding the resolution of data collected (> 20 000 km lines planned) but also adding additional methodologies (magnetometer, side scan sonar, vibrocorer and CPT’s).

The data to retrieve over these 2 years will allow to produce a detailed Terrain model supporting a holistic data interpretation, essential for succeeding actions in the pioneering development of floating wind farms offshore Portugal.

This comprehensive geophysical and geotechnical characterization represents a pioneering effort in Portugal's energy transition, providing crucial data for the sustainable development of offshore wind energy and potentially serving as a model for similar initiatives.

This research was funded by PRR funds - RP-C21-i07.01 - Technical studies for offshore energy potential. This work is also supported by the Portuguese Fundação para a Ciência e Tecnologia, FCT, I.P./MCTES through national funds (PIDDAC): UID/50019/2025, UIDB/50019/2020 (https://doi.org/10.54499/UIDB/50019/2020) and LA/P/0068/2020 https://doi.org/10.54499/LA/P/0068/2020).

 

How to cite: Brito, P., Batista, L., Borges, R., Costa, P., Neres, M., Noiva, J., Pereira, Â., Ribeiro, C., Rosa, M., and Terrinha, P.: Geophysical and Geotechnical offshore studies: pioneering contribution to shape Portugal’s wind farm strategy , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19413, https://doi.org/10.5194/egusphere-egu25-19413, 2025.

Sedimentary and crustal thickness constraints are crucial for refining dynamic topographic measurements and evaluating geothermal energy prospectivity. Continental sedimentary and crustal thickness measurements are constrained in this ongoing global study. Here, we present the updated methodology and results. Total sedimentary thickness is accurately constrained via a combination of well data and controlled-source seismic experiments. A minimum curvature gridding algorithm is used to interpolate between sedimentary thickness data points. Crustal thickness, defined as the vertical depth from the sediment-basement interface to the Moho, is derived from the updated sedimentary thickness grid and recently published studies which exploit controlled- and passive-source seismic data to constrain depth to Moho. A grid resolution of 0.03 degrees is found to be essential for capturing fine-scale lateral variations in sedimentary thickness. Resulting sedimentary and crustal thickness estimates are used to improve continental residual elevation constraints, a proxy for dynamic topography. Residual elevation is quantified by isolating and removing isostatic signals arising from sediment loading and crustal heterogeneity, revealing the magnitude of mantle-induced vertical motion at the surface. Our estimates additionally improve predictions of surface heat flow and geothermal gradients, directly informing geothermal energy assessments. Collectively, these datasets can be used to advance our understanding of mantle-lithosphere interactions and sustainable energy resources.

How to cite: Slay, P., Holdt, M., and White, N.: Improved global sedimentary and crustal thickness constraints: Implications for dynamic topography and geothermal resource assessment, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19524, https://doi.org/10.5194/egusphere-egu25-19524, 2025.

Hydrogen use today is mostly as a chemical feedstock, producing ammonia used in fertiliser production amongst other hard to abate uses. Today’s hydrogen is produced directly from hydrocarbons with the resulting CO2 contribution ca 2.4% of global emissions. Hydrogen as a future clean energy vector could see hydrogen demand increase from ca 95 Mt H2 today, to 540 Mt H2 by 2050.

The mass of hydrogen generated within the continental crust is only recently being appreciated as a potential societal resource. Accumulation and preservation of a small portion of the natural hydrogen, in accessible parts of the continental crust, is required. The dominant sources of natural hydrogen are through water-rock reactions with mafic or ultramafic rocks and the radiolysis of water from the radioactive decay of U and Th in rocks.  The timescales and environments that enable significant hydrogen generation occur in geological different terrane. These vary from dominantly Phanerozoic ophiolite complexes; Proterozoic-Phanerozoic alkaline granite complexes; Mesoproterozoic-Phanerozoic large igneous provinces (LIP) to dominantly Archean TTG and greenstone belts. The tectonic evolution in each setting, and capacity to form traps, is required alongside the porosity and permeability history that exposes the rock to water. To form a commercial reserve, an environment that produces and preserves a free gas phase from the ubiquitous water over the timescale of the system is required. Helium (4He) provides an analogue for natural hydrogen behaviour and the processes that control both deep-seated flux to the near surface and gas phase formation. Loss due to microbial utilisation remains a high preservation risk.

C Ballentine, R Karolytė, A Cheng, B Sherwood Lollar, J Gluyas, M Daly. Natural hydrogen resource accumulation in the continental crust, In review

How to cite: Ballentine, C.: The character and habitat of natural hydrogen resource systems , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19964, https://doi.org/10.5194/egusphere-egu25-19964, 2025.

EGU25-20357 | ECS | Posters on site | GD6.1

Surface geochemistry: from oil and gas exploration to natural hydrogen seeps 

Anna Twaróg and Henryk Sechman

The discovery and exploitation of the first natural (white) hydrogen reservoir in Mali has stimulated global interest in this zero-emission energy resource and carrier. Current research worldwide aims to identify its generation sources, occurrence potential, and extraction feasibility. Tools and methods normally used in hydrocarbon exploration are being adapted for this purpose. One such method is the molecular composition analysis of soil gases, a surface geochemical technique. These methods involve detecting and analyzing trace amounts of light hydrocarbons migrating from subsurface accumulations to the surface. Surface geochemical studies have been conducted across all petroleum basins in Poland. In addition to hydrocarbons, other gases, including hydrogen, were routinely analyzed in many soil gas samples. However, hydrogen played a marginal role in interpreting results aimed at identifying subsurface hydrocarbon accumulations. Large datasets containing hydrogen concentrations in soil gases, recorded over the past 35 years across Poland, remain largely unanalyzed and uninterpreted. One such dataset pertains to the Świdwin-Sławoborze area in Western Pomerania, northern Poland. In 1996, 478 soil gas samples were collected from a depth of 1.2 meters in this region. These samples were analyzed chromatographically for hydrocarbons and non-hydrocarbon gases, including hydrogen.

Molecular composition analysis revealed hydrogen in 85% of the samples, with a maximum concentration of 940 ppm. The mean hydrogen concentration (38 ppm) is five times greater than the median (8 ppm), indicating the presence of anomalous values. Hydrogen concentrations exceeding 40 ppm were partly recorded above an oil deposit located in Zechstein Main Dolomite formations. Elevated hydrogen concentrations in these samples correlate with increased levels of C2-C4 alkanes. Additionally, high hydrogen concentrations were observed above tectonic structures, which may indicate hydrogen migration from deeper horizons.

Reanalyzing and reinterpreting archival geochemical data with a focus on hydrogen concentration variations enables the identification of potential hydrogen migration and leakage zones at the surface. Integrating archived geochemical data with terrain morphology (e.g., potential "fairy circle" structures), geological formations, and the distribution of other resources highlights promising anomalous areas. These zones provide a valuable framework for investigating hydrogen origins and migration patterns within the Polish Zechstein Basin, part of the Central European Permian Basin.

The research project was supported by program “Excellence initiative – research university” IDUB for the AGH University of Krakow (project number 6237).

How to cite: Twaróg, A. and Sechman, H.: Surface geochemistry: from oil and gas exploration to natural hydrogen seeps, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20357, https://doi.org/10.5194/egusphere-egu25-20357, 2025.

CC BY 4.0