Presentation type:
EMRP – Earth Magnetism & Rock Physics

EGU26-3917 | Orals | MAL25-EMRP | Louis Néel Medal Lecture

A revolution in rock physics: 4D imaging 

Francois Renard

The ability to establish rheological and fluid‑transport laws in the lithosphere for use in geomechanics and geodynamics models depends on laboratory experiments validated by field observations. In experiments, a key challenge is reproducing the pressure, temperature, and fluid‑chemistry conditions found at depth while acquiring sufficient information inside rock samples to understand and generalize the detailed mechanisms of rock deformation and chemical evolution. Over the past fifteen years, breakthroughs in rock physics have been enabled by experiments conducted at large user facilities such as synchrotron and neutron sources. From shallow subsurface fluid–rock interactions to slow and fast rupture and down to the brittle–ductile transition at the base of the seismogenic zone and deep earthquakes, it is now possible to image geological processes in 4D (3D + time) with unprecedented spatial and temporal resolution in samples large enough to be representative of lithospheric processes.

Recent experiments demonstrate how a porous rock can become clogged and store carbon dioxide, including direct imaging of fluid mixing and precipitate formation, how porosity can be generated at the brittle–ductile transition, altering our view of fluid transfer at the base of the seismogenic zone, and how damage nucleates before and during earthquakes. These findings highlight the importance of dynamic porosity — which controls fluid transport and deformation — and call for integrating more widely this property into large‑scale models of Earth’s crust dynamics.

How to cite: Renard, F.: A revolution in rock physics: 4D imaging, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3917, https://doi.org/10.5194/egusphere-egu26-3917, 2026.

EGU26-21775 | ECS | Orals | MAL25-EMRP | EMRP Division Outstanding ECS Award Lecture

Determining the mechanical properties of heterogeneous rocks from a knowledge of microstructure 

Lucille Carbillet

Rocks can be described as heterogeneous random materials, in the sense that they are composed of multiple domains of different phases. At the scale of a representative elementary volume (REV) — defined as the smallest volume over which measurements yield values representative of the entire rock sample — such heterogeneous materials can be treated as homogeneous and characterized by macroscopic or effective properties. Determining these effective properties is essential for describing geological processes occurring in reservoirs, aquifers, fault zones, and volcanic environments, as well as the structural changes they induce. However, complex interactions among the constituent phases result in a strong dependence of effective properties on nontrivial aspects of the microstructure, in particular for rocks with more than two or three different phases.

Over the past decades, a fruitful approach to investigating the relationship between rock properties and microstructure has involved predicting effective properties directly from microstructural information. This framework enables quantitative links to be established between microstructural evolution and changes in macroscopic properties. Following this rationale, laboratory-prepared synthetic rocks with specifically designed microstructural attributes have proven particularly valuable. Such materials have provided key insights into the influence of microstructure on mechanical properties, using relatively simple single- or two-phase rock analogs first, and synthetic materials with progressively more numerous distinct phases.

Here, I will summarize results we have collected in the past years by systematically investigating how specific microstructural attributes influence the mechanical behaviour of rocks. Compression experiments conducted on monodisperse sintered glass beads samples show that the stress required to reach inelastic deformation decreases when porosity or grain size alone increase. Using bidisperse and polydisperse sintered glass beads samples, we observe that this stress decreases when the degree of polydispersivity increases. In addition, under high-pressure triaxial compression, an increase in the degree of polydispersity alone leads to a transition in damage evolution from localized to more spatially distributed deformation. These results echo observations from shear experiments performed on heterogeneous fault gouges, where the spatial arrangement of weak and strong mineral phases, in addition to their relative proportions, exerts control on frictional properties and damage evolution during shearing.

More recently, we have employed nanoindentation to resolve spatial variations in elastic properties directly at the grain and crystal scale in natural rocks, allowing for the mechanical characterization of individual phases and quantification of mechanical heterogeneity at the bulk sample scale. These measurements will hopefully provide input parameters for the development and calibration of increasingly realistic synthetic rocks.

How to cite: Carbillet, L.: Determining the mechanical properties of heterogeneous rocks from a knowledge of microstructure, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21775, https://doi.org/10.5194/egusphere-egu26-21775, 2026.

In the Chundi–Malakonda–Ayyavaripalle region of the Nellore Schist Belt, part of the Dharwar Craton, six north-south (N–S) trending, elongated Banded Magnetite Quartzite (BMQ) bands have been identified. These bands are exposed within meta-rhyolite and quartzite formations and are associated with biotite–muscovite schist. The BMQs vary in width from 20 to 40 meters and extend in length from 1.5 to 4.5 kilometres. ​ High-resolution aeromagnetic surveys with a terrain clearance of 80 meters have revealed significant magnetic anomalies over the study area (source: https://geodataindia.gov.in). These anomalies range from –3,900 to +5,000 nanoteslas (nT), indicating a high concentration of magnetic minerals within the exposed BMQs, designated as Bands 1 to 6. In addition to these exposed bands, a concealed, parallel, N–S trending BMQ band has been identified through detailed analysis of aeromagnetic data. 2D and 3D Interpretation of the magnetic anomalies suggests that meta-rhyolites exist up to an average depth of 250 m from the surface and might be associated with BIF bands at depth. This depth extent highlights the substantial vertical continuity of the magnetite-rich formations in the region. The integration of geological mapping and aeromagnetic data provides a comprehensive understanding of subsurface geology, highlighting the potential for significant mineralization within the Nellore Schist Belt.

How to cite: Dharavathu, S., Kosuri, S. K., Vappangi, P. K., and Kumar, P.: Unveiling concealed Banded Magnetite Quartzites (BMQs) through high-resolution aeromagnetic surveys: New insights from the Nellore Schist belt of Eastern Dharwar Craton, India, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2063, https://doi.org/10.5194/egusphere-egu26-2063, 2026.

Within the comprehensive framework of the Sun–Earth system, plasma environments exhibit an exceptionally wide range of physical conditions. These encompass the ultra-high-temperature, high-pressure, and high-density liquid metallic outer core of Earth, which generates the geomagnetic field through the geodynamo process; the tenuous, partially ionized ionosphere; and the magnetosphere, which provides essential shielding against energetic cosmic and solar radiation while exerting substantial influence on human technological systems, most notably microwave communication infrastructure. In addition, transient ultra-high-temperature plasmas generated by solar flares and coronal mass ejections (CMEs) represent the primary drivers of disturbed space electromagnetic environments, as they propagate through interplanetary space and subsequently interact with Earth's magnetosphere.Although prior research has extensively employed the first-principles quantum Monte Carlo method coupled with the lattice Boltzmann approach (FPQM-LBM) to address various theoretical and computational aspects of plasma behavior in this context, no existing modeling framework has successfully integrated — within a single consistent methodology — the extreme conditions of the Earth's outer core plasma, the low-density ionospheric plasma, the magnetospheric plasma, and the highly energetic, transient flare/CME plasmas. As a result, a unified and comprehensive understanding of particle transport mechanisms and internal structural properties across the full spectrum of plasma regimes in the Sun–Earth system remains elusive.The present study aims to address this critical gap by developing novel theoretical frameworks and advanced computational methodologies for elucidating the particle migration mechanisms and structural characteristics of space electromagnetic plasmas throughout the panoramic Sun–Earth system. To this end, we will enhance the first-principles quantum Monte Carlo–lattice Boltzmann method (FPQM-LBM) to establish robust techniques capable of modeling particle transport under the complex electromagnetic conditions prevailing in space environments. The improved FPQM-LBM framework will be systematically applied to simulate particle dynamics across the aforementioned plasma regimes — namely, the ultra-high-temperature/pressure/density outer core plasma, the low-density ionosphere, the magnetosphere, and transient flare/CME plasmas — with particular emphasis on ionic characteristics, microstructural evolution, fine-scale particle transport processes, internal structural transformations, and the response of plasma properties to external electromagnetic perturbations. The anticipated results are expected to furnish a solid theoretical foundation and valuable predictive capabilities for advancing solar–terrestrial space physics and enhancing electromagnetic monitoring and forecasting in space weather research.

How to cite: Zhu, B.: Theoretical Foundations and Methodological Developments in the Study of Particle Transport Mechanisms and Microstructural Evolution Employing the Hybrid Quantum Monte Carlo–Boltzmann Transport Model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3254, https://doi.org/10.5194/egusphere-egu26-3254, 2026.

EGU26-5611 | Posters virtual | VPS29

Improving GIC modelling and validation with high-quality information on power network parameters 

Ciaran Beggan, Gemma Richardson, and Ewelina Lawrence

Space weather can affect the operation of high voltage AC transformers in power grids by applying an offset DC current during periods of heightened geomagnetic activity. Modelling GIC requires knowledge of magnetic field variation, the response of the local subsurface geoelectric field (related to conductivity) and a representation of the connections between transformers and various resistance parameters of the power network. Presently, in Britain, the largest uncertainty in this chain applies to the resistance parameters of the network, as these values come from open-source data which are known to have many approximations.

Recent work with a transmission network operator in the UK has provided us with an improved dataset of resistance parameters of transformers, power lines and substation grounding. The grounding resistance at electrical substations has not been known before and so historically was set at 0.5 Ω in our models. The new dataset of 110 sites around central Scotland reveals substation grounding resistance varies from 0.04 Ω to 11.7 Ω with a mean of 0.54 Ω but a median of 0.2 Ω. Combined with line and transformer resistance information, we have created an improved representation of the power grid in Scotland.

Using GIC measurements from three sites (Torness, Strathaven and Neilston) for the largest geomagnetic storms in the past 25 years (October 2003, September 2017 and May 2024), we are able to validate the new model, demonstrating its improved accuracy.

The new model demonstrates that our previous assumptions of grounding resistance were too high but our estimate of line resistance was too low, thus balancing out the overall GIC magnitude on average. However, in detail, some locations show large differences in GIC compared to the original model. This highlights the importance of using accurate resistance information to correctly capture GIC.

How to cite: Beggan, C., Richardson, G., and Lawrence, E.: Improving GIC modelling and validation with high-quality information on power network parameters, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5611, https://doi.org/10.5194/egusphere-egu26-5611, 2026.

During intense solar atmospheric activity—such as major solar flares and geomagnetic storms—magnetic energy is converted into plasma kinetic and thermal energy through three-dimensional turbulent magnetic reconnection within large-scale, extended current sheets. This process releases enormous amounts of stored energy, often accompanied by the rapid ejection of high-energy particles into interplanetary space. These high-energy particles include electrons, protons, helium nuclei, and heavier ions, forming a complex multi-component, multi-abundance, and multi-isotopic population. Their energies span from ~100 keV to ~100 MeV and even into the GeV range, making them a primary driver of space weather hazards. Understanding the sources and acceleration mechanisms of these particles remains one of the most critical challenges in space weather research. Previous studies have shown that high-energy particle acceleration is highly complex, involving multiple species, a variety of mechanisms, and interactions across scales. It remains an open and challenging problem in solar and plasma physics. This paper provides a systematic review and forward-looking perspective on recent advances in high-energy particle acceleration during the fine-scale evolution of large-scale current sheets. The discussion is organized around three key pillars: theory, observations, and numerical simulations. First, we summarize the turbulence-fractal model as it applies to typical solar atmospheric events. We focus on acceleration mechanisms in turbulent magnetic reconnection within large spatiotemporal current sheets, with particular emphasis on: Turbulent (second-order) Fermi acceleration, Turbulent shock acceleration, and Turbulent wave-particle resonant acceleration. These mechanisms operate synergistically in the turbulent environment generated by reconnection, enabling efficient energy transfer to particles. Second, we review recent progress in coupling macroscopic (hydrodynamic and magnetohydrodynamic) dynamics to microscopic kinetic processes in high-energy particle acceleration. This includes multi-scale modeling of turbulence, reconnection, and particle transport. Finally, we outline promising future research directions, including improved multi-spacecraft observations, higher-resolution simulations that incorporate kinetic effects, and integrated models that bridge MHD turbulence and particle-in-cell approaches. We also highlight several urgent unresolved issues, such as the relative contributions of different mechanisms across energy regimes, the role of fractal structures in particle trapping and escape, and the origin of observed abundance enhancements in heavy ions. This review synthesizes recent theoretical, observational, and computational developments to provide a comprehensive framework for understanding high-energy particle acceleration in large-scale turbulent current sheets, with implications for solar flares, space weather forecasting, and broader astrophysical plasma processes.

How to cite: Zhu, B.: Research Progress on SEPs on the Fine Structures of the Large Temporal-spatial Current Sheets in Solar Flares/CMEs, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6969, https://doi.org/10.5194/egusphere-egu26-6969, 2026.

EGU26-8141 | ECS | Posters virtual | VPS29

A Late Holocene Paleomagnetic Record from Lago del Desierto, Southern Patagonia (Argentina) 

Romina Valeria Achaga, Claudia Susana Gabriela Gogorza, Maria Alicia Irurzun, Christian Ohlendorf, Torsten Haberzettl, and Bernd Zolitschka

Lago del Desierto (49°02′S, 72°51′W) is located in a climatically sensitive sector near the Southern Patagonian Ice Field (Argentina). Three sediment cores collected from two sites in the lake were analyzed using a multi-proxy approach to reconstruct past environmental variability (Kastner et al., 2010). Numerous turbidites were identified in the sedimentological record. After excluding these event layers, a new age–depth model was developed for the first 3 sections of the core DES05-3 (289 cm), and paleosecular variations (PSV) were reconstructed for the interval between ~1000 and 3500 cal. BP.

Standard paleomagnetic measurements (alternating-field demagnetization) were performed on 125 samples from the same core. In addition, rock-magnetic measurements, including Anhysteretic Remanent Magnetization (ARM, 100 mT peak AF, 0.05 mT DC field), Isothermal Remanent Magnetization (IRM, acquisition up to 1.5 T and backfield curves), hysteresis loops and thermomagnetic analyses, were applied to extract complementary paleoenvironmental information from the sediment cores.

Rock-magnetic measurements indicate that the magnetic mineralogy is dominated by a low-coercivity component (magnetite-type), accompanied by a secondary high-coercivity fraction (hematite/goethite-type). This downcore distribution mirrors the paleoenvironmental shift described by Kastner et al. (2010): the lower part of the sequence shows an enhanced contribution of high-coercivity Fe oxides, consistent with more stable and chemically weathered catchment conditions. In contrast, the upper part shows an increasing dominance of detrital magnetite, indicating strengthened minerogenic supply and enhanced erosion, matching the onset of warmer conditions and glacier retreat during the Medieval Climate Anomaly as inferred from geochemical and lithological proxies. This agreement between magnetic and non-magnetic sediment parameters suggests coherent changes in the provenience of the sediment and in catchment dynamics over the last millennia. As expected from the catchment instability and the numerous turbidites in the upper part of the sequence, this interval could not be used for PSV reconstruction due to its discontinuous directional record. In contrast, samples from the lower part (~1000–3500 cal. BP) provided a continuous sequence suitable for paleosecular variation analysis. Although samples from this unit were not completely demagnetized at 100 mT, due to the presence of a high-coercivity component, magnetization directions consistently decayed toward the origin with high precision. Characteristic remanent magnetization (ChRM) directions were determined using principal component analysis, with maximum angular deviation (MAD) values below 2.5° for all non-turbidite samples. The resulting PSV record compares well with geomagnetic field models and other Patagonian paleomagnetic reconstructions. Inclination values range from −40° to −70°, displaying coherent directional variability over the last ~3500 years.

References:
Kastner, S., Enters, D., Ohlendorf, C., Haberzettl, T., Kuhn, G., Lücke, A., Mayr, C., Reyss, J.-L., Wastegård, S., & Zolitschka, B. (2010). Reconstructing 2000   years of hydrological variation derived from laminated proglacial sediments of Lago del Desierto at the eastern margin of the South Patagonian Ice Field, Argentina. Global and Planetary Change, 72(3), 201-214. https://doi.org/10.1016/j.gloplacha.2010.04.007

How to cite: Achaga, R. V., Gogorza, C. S. G., Irurzun, M. A., Ohlendorf, C., Haberzettl, T., and Zolitschka, B.: A Late Holocene Paleomagnetic Record from Lago del Desierto, Southern Patagonia (Argentina), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8141, https://doi.org/10.5194/egusphere-egu26-8141, 2026.

EGU26-8566 | Posters virtual | VPS29

Pc3 geomagnetic pulsations excited by earthquakes and their commonality with solar wind-originated Pc3 

Toshihiko Iyemori, Tadashi Aoyama, and Yoshihiro Yokoyama

The source of compressional Pc3 magnetic pulsations has been considered to be the plasma process in the solar wind or in the magnetosphere. However, we found some strong inland earthquakes that occur on the dayside also excite Pc3s. The Lamb waves generated by the January 2022 Tongan undersea volcanic eruption are also believed to have excited large amplitude and short period compressional Pc3 geomagnetic pulsations in the dayside plasmasphere (Iyemori et al., 2025). Increases in power spectral density (PSD) in the Pc3 frequency band were observed 10-30 minutes after the origin time of large inland earthquakes (M>6.5) during the daytime (10-14 LT). During these large earthquakes, seismic waves with period of 10-30 seconds propagate far away (even more than several thousand km), causing slight fluctuations in the orientation of magnetometer sensors, resulting in apparent Pc3-like fluctuations. To avoid such sensor tremor effect, we analyzed the total force of magnetic field, or analyzed comparing with seismometer data. We also used the Swarm satellite observation. The PSD of Pc3s caused by earthquakes or by Lamb wave show many spectral peaks having interval of 3-5 mHz, and this is similar with the characteristic reported by, for example, Samson et al. (1995) for normal, i.e., solar wind origin Pc3s. In this paper, we will also show the commonality between the Pc3s caused by earthquakes or Lamb waves and those originated from the solar wind and discuss what the commonality means.

How to cite: Iyemori, T., Aoyama, T., and Yokoyama, Y.: Pc3 geomagnetic pulsations excited by earthquakes and their commonality with solar wind-originated Pc3, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8566, https://doi.org/10.5194/egusphere-egu26-8566, 2026.

EGU26-8852 | Posters virtual | VPS29

High-resolution magnetic record of environmental changes during Middle – Late Pleistocene from a loess-palaeosol sequence in NE Bulgaria – pilot data from the LOEs-CLIMBE project 

Diana Jordanova, Bozhurka Georgieva – Ishlyamska, Daniel Veres, Yunus Baykal, Marius Robu, Neli Jordanova, Ulrich Hambach, Daniel Ishlyamski, Dimo Dimov, Andrew Trott, and Guido Wiesenberg

Continental sedimentary sequences of alternating loess and palaeosol horizons preserve detailed records of past global climate changes during the Pleistocene. Obtaining deeper and genuine knowledge on the history of past climates using proxy data depends on interdisciplinary approaches, novel techniques and thinking “out-of-the-box”. The LOEs-CLIMBE team members gather around this concept and present here the first pilot magnetic data from the Kolobar loess-palaeosol section in NE Bulgaria. The 25 m thick section is exposed in an active quarry and was sampled at 2-cm-resolution, covering the Holocene soil, seven palaeosol units and loess horizons L1 to L7 of varying thicknesses. New high resolution magnetic susceptibility data, delineates palaeosol horizons with high values of mass specific magnetic susceptibility except the special case of fourth palaeosol S4, showing no magnetic enhancement as compared to the underlying thin loess. Such depletion of pedogenic magnetic enhancement in paleosol units from the Lower Danube area is rarely reported. This phenomenon will be further examined by detailed magnetic and colorimetric methods. The strongest pedogenic magnetic signal is observed in the three youngest palaeosol units S1, S2 and S3, tentatively related to the interglacial stages MIS 5, MIS 7 and MIS 9. The weakest magnetic susceptibility is typical for the younger part of the loess unit L2, punctuated by the signal of a tephra layer, which is a widespread chronostratigraphic marker in the region.  This research is carried out and financed within the framework of the second Swiss Contribution MAPS, LOEs-CLIMBE project № IZ11Z0_230102.

How to cite: Jordanova, D., Georgieva – Ishlyamska, B., Veres, D., Baykal, Y., Robu, M., Jordanova, N., Hambach, U., Ishlyamski, D., Dimov, D., Trott, A., and Wiesenberg, G.: High-resolution magnetic record of environmental changes during Middle – Late Pleistocene from a loess-palaeosol sequence in NE Bulgaria – pilot data from the LOEs-CLIMBE project, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8852, https://doi.org/10.5194/egusphere-egu26-8852, 2026.

EGU26-9301 | ECS | Posters virtual | VPS29

The influence of the heterogeneity (stratification) of the outer core fluid on the variation of the geomagnetic field 

Shichao Wang, Yongbing Li, Bojing Zhu, Yang Zhao, Qian Wang, and Hanfen Liu

The Earth's magnetic field is divided into internal and external sources, with the internal field including the main magnetic field, the crustal magnetic field, and the induced magnetic field. Among these, the main magnetic field accounts for approximately 95% of the Earth's total magnetic field. Data from paleomagnetic records in rocks, various geomagnetic observatories, and satellites indicate that the main magnetic field exhibits westward drift, polarity reversals, intensity decay, and brief geomagnetic excursions at the core-mantle boundary. To explain these phenomena, several models have been proposed in previous studies. The prevailing view is that the outer core is composed of liquid metal, and the Earth's main magnetic field is generated by the turbulent fluid motion of this liquid metal, influenced primarily by factors such as its composition and properties, thermal convection, Lorentz force, and Coriolis force. Considering the strong Coulomb forces between electrons and ions, previous research has usually treated the electrons and ions in the outer core's metallic fluid as a unified component, greatly simplifying the study and achieving satisfactory results. However, existing studies have not taken into account the differences in motion between ions and electrons under the dynamics of the outer core, the resulting spatial distribution differences of electrons and ions in the outer core, or the impact of these differential distributions on the Earth's main magnetic field. In view of this, This paper studies the effect of the factors generating outer core dynamics on the distribution of electrons and ions in the outer core. It examines the distribution of electrons and ions in the outer core space under equilibrium conditions and estimates their contribution to Earth's main magnetic field. Then, by changing parameter conditions (such as temperature gradients) and adding convective terms (non-equilibrium state), the calculations are redone. These results are used to explain changes in Earth's magnetic field.

How to cite: Wang, S., Li, Y., Zhu, B., Zhao, Y., Wang, Q., and Liu, H.: The influence of the heterogeneity (stratification) of the outer core fluid on the variation of the geomagnetic field, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9301, https://doi.org/10.5194/egusphere-egu26-9301, 2026.

EGU26-10911 | Posters virtual | VPS29

Mineralogical Drivers of Ground Failure in Neogene Sediments: a Case Study from Northwest Bulgaria 

Zornitsa Dotseva, Dian Vangelov, and Tsveta Stanimirova

The stability of critical infrastructure in Northwest Bulgaria (Western Moesian Platform) could be compromised by ground instability within Neogene sediments that cover the region. This is evidenced by the collapse of the I-1 national road near Dimovo town in 2006, which involved vertical displacements of 3–4 meters. The purpose of this study is to identify the underlying geological drivers of this failure and to evaluate the specific hazard in the area resulting from the interaction between the sediments and the local environmental conditions. We hypothesize that the instability is not merely a result of conventional failure mechanisms but is governed by an anomalous mineralogical composition, specifically by the presence of aragonite and gypsum layers, which could create a dual hazard.

To elucidate geological drivers, we employed a methodology that integrates field mapping and sampling with laboratory analyses. Samples from the Neogene sediments in the area of 2006 damage underwent mineralogical analyses using X-ray diffraction (XRD) and Scanning Electron Microscopy (SEM) to determine phase composition and morphology. These analyses were coupled with X-ray fluorescence (XRF) for chemical profiling and standard geotechnical testing to determine grain size distribution, Atterberg limits, and Activity index according to Skempton’s classification.

The analysis reveals a heterogeneous sediment succession with the presence of inorganic clays with high plasticity. The XRD and SEM results identified a mineralogical anomaly where the high concentrations of metastable, acicular aragonite coexist with active swelling phyllosilicates (smectite/illite). Furthermore, various amounts of gypsum were detected in some of the samples, indicating an evaporitic paleoenvironment. Geotechnically, these materials exhibit extreme reactivity. Liquid limits range from 34.85% to 67.88%, and plasticity indices reach up to 47.39%. The Activity index peaks at 2.00, categorizing the sediments as "highly active" and prone to volume change driven by moisture variations.

The study concludes that ground failure is a direct consequence of a synergistic hydro-chemo-mechanical mechanism driven by the sediments' mineralogy. The specific aragonite fabric allows rapid water infiltration, triggering the hydration of smectites that could lead to loss of shear strength. Simultaneously, gypsum dissolution could create secondary porosity, reduce effective stress, and release sulfate ions, which could pose a potential chemical hazard to concrete foundations through sulfate attack. Furthermore, the high silt content facilitates internal erosion and possible piping through fracture networks, which could explain the sudden loss of support and large vertical displacements observed in the 2006 case. These findings imply that standard geotechnical data alone are insufficient for risk assessment in this region. Effective mitigation strategies must integrate mineralogical analysis to address both the physical swelling and the chemical durability risks.

Acknowledgements: This research was funded by the European Union-NextGenerationEU, through the National Recovery and Resilience Plan of the Republic of Bulgaria, Project No BG-RRP-2.004-0008-C01.

How to cite: Dotseva, Z., Vangelov, D., and Stanimirova, T.: Mineralogical Drivers of Ground Failure in Neogene Sediments: a Case Study from Northwest Bulgaria, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10911, https://doi.org/10.5194/egusphere-egu26-10911, 2026.

EGU26-14934 | ECS | Posters virtual | VPS29

Effects of the Historical Geomagnetic Field on Earth's Energetic Particle Environment: Magnetic Anomalies and Auroral Regions  

Kirolosse Girgis, Maximilian Arthus Schanner, Sanja Panovska, and Akimasa Yoshikawa

Three centuries ago, auroral emissions could be observed over the Korean sector, where the West Pacific Anomaly (WPA) coexisted with the South Atlantic Anomaly (SAA). To investigate this phenomenon, the present study builds upon our recent numerical simulations of the inner proton radiation belt [Girgis et al., JSWSC (2021), Girgis et al., SW (2023,2024)], in which we examined the effects of space weather on the near-Earth particle environment. Here, we extend our modeling framework to explore the historical distribution and state of the radiation environment. A key aspect of this research is the incorporation of a geomagnetic field configuration representative of the year 1650, and the comparison of the resulting particle environment with that derived from contemporary magnetic field models.  The primary objective is to model the near-Earth particle environment in a manner that enables future coupling with atmospheric models, while also accounting for the influence of external space weather conditions. A comprehensive understanding of both the present-day and historical particle dynamics in the near-Earth environment is essential for predicting radiation conditions relevant to low Earth orbit (LEO) missions and for assessing the potential impact on Earth’s atmosphere. 

How to cite: Girgis, K., Arthus Schanner, M., Panovska, S., and Yoshikawa, A.: Effects of the Historical Geomagnetic Field on Earth's Energetic Particle Environment: Magnetic Anomalies and Auroral Regions , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14934, https://doi.org/10.5194/egusphere-egu26-14934, 2026.

EGU26-18706 | ECS | Posters virtual | VPS29

SwarmDF: A toolbox for analysing high-latitude ionospheric electrodynamics 

Margot Decotte, Karl M. Laundal, and Fasil T. Kebede

The Swarm Data Fusion (SwarmDF) toolbox is designed as an easy-to-use Python module for analysing the local electrodynamics of the high-latitude ionosphere by combining measurements from ESA’s Swarm satellites with additional ionospheric and thermospheric datasets. Given a Swarm satellite ID, a regional grid, and a time interval, the toolbox automatically retrieves and combines available observations from SuperDARN, SuperMAG, Iridium/AMPERE, and Swarm electromagnetic field measurements. SwarmDF uses the local mapping of polar ionospheric electrodynamics (Lompe) technique to reconstruct two-dimensional maps of key electrodynamic parameters in the vicinity of the Swarm satellite tracks. To assess and quantify reconstruction performance, SwarmDF integrates the LompeOSSE Python module, which generates controlled synthetic electrodynamics datasets based on Gamera simulations and enables systematic comparisons with the toolbox outputs under different data availability and configuration scenarios. Featuring a user-friendly graphical interface, SwarmDF simplifies data handling and model setup for high-latitude ionospheric electrodynamic studies using Swarm observations.

How to cite: Decotte, M., Laundal, K. M., and Kebede, F. T.: SwarmDF: A toolbox for analysing high-latitude ionospheric electrodynamics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18706, https://doi.org/10.5194/egusphere-egu26-18706, 2026.

EGU26-21147 | ECS | Posters virtual | VPS29

Dimensionality Analysis of the Iberian Pyrite Belt Lithosphere derived from the Magnetotelluric Impedance Tensor. 

Pedro Baltazar-Soares, Francisco José Martinéz-Moreno, Lourdes Gonzaléz-Castillo, Jesús Galindo-Zaldívar, Fernando Monteiro Santos, Antonio Mateus, and Luis Matias

The Iberian Pyrite Belt (IPB) hosts one of the largest concentrations of massive sulfide deposits in Europe, yet its lithosphere architecture remains incompletely understood. In this study, we employ magnetotelluric (MT) impedance tensor data to investigate the dimensionality and structural characteristics of the IPB crust. The analysis combines two complementary approaches: WAL invariants, computed from the MT impedance tensor using the Waldim code (Martí et al., 2013), which are scalar, rotation invariant quantities providing a robust, frequency dependent measure of three-dimensionality and highlighting anisotropic features in the conductivity distribution; and the Phase Tensor, following the methodology of Caldwell et al. (2004), which offers distortion free insights into the orientation and geometry of regional conductive structures. Integrating these methods enables a systematic dimensional analysis of the impedance tensor, revealing lateral heterogeneities, preferred orientations of conductive features, and depth dependent variations in lithospheric responses.

The results demonstrate that WAL invariants and Phase Tensor analysis together allow the separation of near surface distortions from deeper geoelectric structures, providing a robust framework for characterizing the lithospheric architecture of the IPB. This study highlights the enhanced resolution and robustness achieved by complementing the tensor based analysis of MT data with invariant derived quantities that provide rotationally independent measures of three-dimensionality and anisotropy.

Consequently, this dimensional and structural assessment constitutes a critical prerequisite for subsequent MT data inversion, as it provides essential constraints on model dimensionality, structural orientation, and the treatment of near surface distortion. By supporting the choice between 2D and 3D inversion strategies, the proposed framework enhances the stability of the inversion process, increases the reliability of the conductivity distributions, and ensures greater geological consistency of the resulting models.

Acknowledgment

This work is supported by FCT, I.P./MCTES through national funds (PIDDAC): LA/P/0068/2020, https://doi.org/10.54499/LA/P/0068/2020,UID/50019/2025,  https://doi.org/10.54499/UID/PRR/50019/2025, UID/PRR2/50019/2025

References

Caldwell, T.G., Bibby, H.M. and Brown, C. (2004). The magnetotelluric phase tensor. Geophysical Journal International, 158: 457-469. https://doi.org/10.1111/j.1365-246X.2004.02281.x

Castro, C., Hering, P., Junge, A. (2020). FFMT: a MATLAB-based toolbox for Magnetotellurics (MT). 10.13140/RG.2.2.12465.92007.

F. E. M. Lilley. (1998). Magnetotelluric tensor decomposition; Part, Theory for a basic procedure. Geophysics; 63 (6): 1885–1897. doi: https://doi.org/10.1190/1.1444481.

Martí, A., Queralt, P., Ledo, J., Farquharson, C. (2010). Dimensionality imprint of electrical anisotropy in magnetotelluric responses, Physics of the Earth and Planetary Interiors, Volume 182, Issues 3–4, 2010, Pages 139-151, ISSN 0031-9201. https://doi.org/10.1016/j.pepi.2010.07.007.

Martí, A., Queralt, P., Ledo, J. (2013). WALDIM: A code for the dimensionality analysis of magnetotelluric data using the rotational invariants of the magnetotelluric tensor. Computers & Geosciences. 2295-2303. 10.1016/j.cageo.2009.03.004

Miensopust, M. P. (2017). Application of 3-D electromagnetic inversion in practice: Challenges, pitfalls and solution approaches. Surveys in Geophysics, 38(5), 869–933. https://doi.org/10.1007/s10712-017-9435-1.

Vozoff, K. (1991). The magnetotelluric method: Electromagnetic methods. In M. N. Nabighian (Ed.), Applied Geophysics (pp. 641–712).

Kelbert, A., Meqbel, N., Egbert, G. D., & Tandon, K. (2014). ModEM: A modular system for inversion of electromagnetic geophysical data. Computers & Geosciences, 66, 40–53. https://doi.org/10.1016/j.cageo.2014.01.010.

How to cite: Baltazar-Soares, P., Martinéz-Moreno, F. J., Gonzaléz-Castillo, L., Galindo-Zaldívar, J., Monteiro Santos, F., Mateus, A., and Matias, L.: Dimensionality Analysis of the Iberian Pyrite Belt Lithosphere derived from the Magnetotelluric Impedance Tensor., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21147, https://doi.org/10.5194/egusphere-egu26-21147, 2026.

EGU26-3508 | Posters virtual | VPS30

Subsurface structural mapping using high-resolution gravity data and advanced processing techniques in the Ouarzazate Basin, Southern Morocco. 

Brahim Bouali, Fatima-Zahra Tabayaoui, Hassan Sahbi, Ahmed Manar, Abderrahime Nouayti, Mustapha Boujamaoui, and Nour eddine Berkat

This study investigates the deep structure of the Ouarzazate Basin, located between the Central High Atlas and the Anti-Atlas, using gravity data analysis. Gravimetric methods were applied to map subsurface structural lineaments beneath the sedimentary cover. The resulting structural map reveals that the basin is mainly controlled by ENE-WSW oriented faults, with subordinate E-W and NE-SW trends related to Variscan deformation, Triassic-Jurassic rifting, and Atlas tectonic inversion. Positive gravity anomalies show preferential NE-SW and E-W orientations and are linked to the structural configuration of the Central High Atlas, which acted as a major source area for the basin. The identified fault systems and compressional structures in the Central High Atlas and Anti-Atlas are consistent with the regional geodynamic evolution. These results highlight the strong tectonic connection between the Ouarzazate Basin and adjacent Atlas basins, particularly the Central High Atlas, and provide new insights into the basin’s geodynamic development.

How to cite: Bouali, B., Tabayaoui, F.-Z., Sahbi, H., Manar, A., Nouayti, A., Boujamaoui, M., and Berkat, N. E.: Subsurface structural mapping using high-resolution gravity data and advanced processing techniques in the Ouarzazate Basin, Southern Morocco., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3508, https://doi.org/10.5194/egusphere-egu26-3508, 2026.

EGU26-5809 | ECS | Posters virtual | VPS30

Rotation of tectonic blocks controlled by strike-slip component along the Zahedan fault, Iran 

Zahra Paktarmani, Andrzej Konon, and Mateusz Mikołajczak

The Zahedan fault zone in Iran constitutes an active tectonic zone characterised by a complex network of strike-slip faults that dominate the local deformation pattern. This area is located within a large-scale transpressional shear zone accommodating relative motion between the Central East Iranian block and the Afghan Helmand block. The region provides a natural laboratory for investigating the relationship between strike-slip faulting and tectonic blocks rotated around vertical axes.

We present herein, based on high-resolution 2025 Airbus satellite imagery and cartographic and geophysical data, a new strike-slip fault pattern that facilitated the development of the rotated tectonic blocks.

Our observations show that the major strike-slip fault zones are accompanied by dense networks of second-order faults, including single sets of antithetic and synthetic strike-slip faults, conjugate strike-slip fault sets, restraining and releasing stepovers, and thrust faults. In several sectors along the major faults occur the zones of deformation consisting of the rotated tectonic blocks. The scale, orientation, and spatial organisation of the mapped structures indicate that block rotation is controlled by the interaction between major strike-slip faults and subsidiary fault networks.

The individual second-order antithetic faults display that these faults commonly accommodate small displacements, but the faults play a critical role in allowing internal deformation within blocks and facilitate the progressive block rotation. The sense of movements along the major fault and the antithetic strike-slip faults bounding the tectonic blocks allows us to consider the structures as the blocks rotated around vertical axes in a domino-like orientation. Recognised examples of structures show that some rotating blocks are rigid, with no evidence of significant internal deformation, while other rotating blocks exhibit strong internal deformation.

Understanding these spectra of behaviours and the determination of the relationships between them will improve our knowledge of fault interaction processes in eastern Iran and related patterns of seismicity, and it also has implications for seismic hazard assessment in active transpressional settings.

How to cite: Paktarmani, Z., Konon, A., and Mikołajczak, M.: Rotation of tectonic blocks controlled by strike-slip component along the Zahedan fault, Iran, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5809, https://doi.org/10.5194/egusphere-egu26-5809, 2026.

Charnockite is generally regarded as a product of high-temperature melting; however, its specific origin, generation, and preservation mechanisms, as well as its relationship to high-grade metamorphism or deep crustal reworking, remain poorly constrained. During the early Paleozoic, the South China Block underwent intense orogeny that resulted in significant crustal shortening and thickening, subsequently inducing widespread anatexis and extensive S-type granites. This study identifies ~431 Ma charnockites containing granulitic enclaves that were exposed in the Yunkai massif, providing key insights into the early Paleozoic crustal reworking and deep crustal melting behaviors in South China. The body displays A-type characteristics with crustal reworking zircon isotopic features (δ18O = 8.0–9.8 ‰; εHf(t) = - 11.5 to - 3.4). The charnockite and its enclaves show identical mineral assemblages and comparable orthopyroxene chemical compositions. The two anhydrous minerals of orthopyroxene and garnet are identified as of peritectic and magmatic origins given their textural features and geochemical compositions. Moreover, petrographic observations and bulk geochemical data argue that the peritectic minerals were derived from the entrainment of their granulitic sources. Crystallization phase modeling indicates orthopyroxene would have been completely hydrated and formed biotite when water contents exceed ∼0.3 wt.% near the solidus. Water-in-zircon analysis and thermodynamic modeling indicate low magma water contents (∼0.15 wt.%; 135 ppm, zircon water medians) for the Gaozhou charnockite from early crystallization to final solidification. CO2‐rich fluids flushed the charnockite reservoir further contributing to the stabilization of the orthopyroxene. Accordingly, the Yunkai charnockite reveals deep crustal melting processes involving anhydrous minerals entrained in a low-water environment. This low-water environment correlates with high-temperature melting of granulite-facies rocks in the lower crust and the presence of CO₂-rich fluids within the system. Regional magmatic-metamorphic-tectonic data indicate that the formation of the Yunkai A-type charnockite occurred within a post-orogenic extension regime, representing the peak of intracrustal reworking in South China.

How to cite: yang, H. and Yao, J.: Formation of A-type charnockite and constraints on deep crustal anatexis in early Paleozoic orogen, South China, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8520, https://doi.org/10.5194/egusphere-egu26-8520, 2026.

EGU26-12696 | ECS | Posters virtual | VPS30

Constraining Early Miocene Reactivation of the Main Mantle Thrust (Swat Valley, Pakistan) through Integrated Structural and Thermochronologic Analysis 

Daniel Ricardo Hernández Chaparro, Claudio Faccena, Valerio Olivetti, Giuditta Fellin, and Humaad Ghani

Unravelling the tectonic evolution of collisional orogens and the forces driving the exhumation of high-grade metamorphic rocks requires constraining the kinematics and timing of major fault systems. The Main Mantle Thrust (MMT) in the Swat Valley (northern Pakistan) marks the Eocene suture between the Indian Plate and the Kohistan–Ladakh Island Arc. Its later reactivation is critical yet debated, with models ranging from dominantly dextral strike-slip faulting with minor normal offset (typically less than a few meters) to significant normal faulting facilitating regional exhumation of high-grade metamorphic rocks. This research integrates structural geology with a new, multi-method low-temperature thermochronology dataset—including zircon and apatite (U–Th)/He and apatite fission-track ages—to contribute to this debate. Structural analysis of over 150 kinematic indicators collected along the MMT and its footwall shows that the MMT experienced semi-ductile to brittle reactivation dominated by top-to-the-north normal faulting. Structures formed under greenschist- to sub-greenschist facies conditions (e.g., C′ shear bands) in the footwall record progressive exhumation, with purely brittle cataclastic deformation marking the final stages. Our new thermochronometer dateset includes zircon (U–Th)/He (ZHe) single-grain ages (14.9 ± 1.2 to 24.4 ± 2.0 Ma), apatite (U–Th)/He (AHe) single-grain ages (7.6 ± 0.4 to 15.9 ± 1.0 Ma), and apatite fission-track (AFT) central ages (15.3 ± 2.4 to 16.4 ± 3.2 Ma). This dataset, alongside its thermal history modelling, reveals a consistent cooling signal across the Swat Valley. Following the Eocene collision and peak metamorphism, a major tectonic shift occurred in the Early Miocene. Our data indicate the onset of rapid cooling at ~20 Ma, with a slightly later initiation at ~18 Ma in the eastern Loe Sar Dome. This distinct phase of rapid cooling records the top-to-the-north normal reactivation of the MMT, which lasted until ~15–14 Ma. Collectively, our results provide structural and timing constraints supporting a model of protracted, normal-sense reactivation of the MMT between ~20 and 15 Ma. This event facilitated the final unroofing of high-grade metamorphic rocks in the Swat Valley. 

How to cite: Hernández Chaparro, D. R., Faccena, C., Olivetti, V., Fellin, G., and Ghani, H.: Constraining Early Miocene Reactivation of the Main Mantle Thrust (Swat Valley, Pakistan) through Integrated Structural and Thermochronologic Analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12696, https://doi.org/10.5194/egusphere-egu26-12696, 2026.

EGU26-16222 | ECS | Posters virtual | VPS30

Quantitative lineament network analysis of a folded crystalline terrain using FracPaQ: The Kadavur Anorthosite Complex, Southern Granulite Terrane 

Aravind Prathapachandran, Arunima Manilal Girija, and R Senthil Kumar

The Kadavur Anorthosite Complex represents a distinctive structural domain within a folded high-grade crystalline terrain, where a massif-type anorthosite body occupies the core of a regional-scale fold and is surrounded by folded quartzite ridges. This study examines the relationship between lineament development and the pre-existing ductile fold architecture through integrated DEM–SRTM data analysis and quantitative lineament network characterisation using FracPaQ. The objective is to assess how fold geometry and lithological contrasts influence the spatial distribution and mechanical behaviour of brittle structures. DEM analysis reveals a coherent folded morpho-structural architecture characterised by a well-defined core, axial-plane domains, and limbs expressed as quartzite ridges. FracPaQ-derived results show that lineaments are non-randomly distributed and define multiple dominant orientation sets, reflecting systematic structural control rather than random patterns. Spatial variations in lineament density and lineament intensity show pronounced localisation within and adjacent to the fold core, whereas lineament attributes vary systematically between the anorthosite-dominated core and the surrounding folded quartzite limbs.

Slip tendency analysis indicates that brittle deformation is predominantly shear-controlled across the study area, while dilation tendency values are generally low to moderate, suggesting a subordinate role for opening-mode fracturing. Lineaments within the anorthosite core are comparatively longer, less densely spaced, and display lower orientation dispersion, reflecting brittle stress accommodation within a mechanically competent lithology. In contrast, lineaments developed in the folded quartzite ridges are shorter, more closely spaced, and strongly influenced by lithological layering and fold-related bending stresses.

Although comparable lineament orientation patterns occur across the fold core, axial planes, and limbs, their geometric characteristics, spatial distribution, and inferred mechanical roles differ significantly, indicating that brittle deformation was modulated by local fold geometry and lithological contrasts. The results indicate a structural association between ductile folding and later brittle deformation; however, the tectonic conditions responsible for anorthosite exhumation cannot be uniquely constrained from the present dataset. This study highlights the importance of domain-specific lineament analysis in folded crystalline terrains and emphasizes the role of inherited ductile architecture in controlling later brittle deformation.

How to cite: Prathapachandran, A., Manilal Girija, A., and Kumar, R. S.: Quantitative lineament network analysis of a folded crystalline terrain using FracPaQ: The Kadavur Anorthosite Complex, Southern Granulite Terrane, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16222, https://doi.org/10.5194/egusphere-egu26-16222, 2026.

EGU26-18367 | ECS | Posters virtual | VPS30

Quantitative Characterization of Fracture Networks Based on Geometric-Topological Integration and Its Application in Hydrocarbon Migration Prediction in the Western Junggar Basin 

Ye Tao, Lijie Cui, Yuxi Niu, Yawen Huang, Song Bai, Guoan Zhao, Paerhati Piluolan, and ying liu

With the continuous advancement of geological research, quantitative analysis of fracture networks has become a crucial research direction in geological exploration and resource development. To overcome the limitations of traditional methods in quantitatively analyzing fault data under complex geological conditions, we adopt a quantitative fracture characterization method based on geometric and topological theories. This study focuses on the overlay analysis of multi-period and multi-layer faults in a typical area of the western Junggar Basin, aiming to reveal their significant role in hydrocarbon exploration. By means of this method, we achieve multi-dimensional automatic quantification of geometric features (including fracture network length, orientation, and Pxy system), as well as node/branch types and topological parameters. Through the construction of a fracture topological network, we can quantitatively analyze the connectivity characteristics of each period and the vertically favorable conduction zones across multiple periods, thereby providing valuable guidance for hydrocarbon migration path prediction.

How to cite: Tao, Y., Cui, L., Niu, Y., Huang, Y., Bai, S., Zhao, G., Piluolan, P., and liu, Y.: Quantitative Characterization of Fracture Networks Based on Geometric-Topological Integration and Its Application in Hydrocarbon Migration Prediction in the Western Junggar Basin, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18367, https://doi.org/10.5194/egusphere-egu26-18367, 2026.

The Achankovil Shear zone (AKSZ), juxtaposing the Trivandrum Granulite Block (TB) and the Madurai Granulite Block (MB) of the Southern Granulite Terrane (SGT), represents a paleo-suture zone related to the late Neoproterozoic to early Cambrian Gondwana assembly (Rajesh et al., 1998; Praharaj et al., 2021). The polyphase deformational history of the Achankovil Shear Zone (AKSZ) reveals progressive transition from a ductile to brittle deformation regime concomitant with high-grade granulite facies metamorphism and subsequent cooling–exhumation of the granulites. Progressive evolution of the state of stress and the variation of crustal dynamics during the ductile to brittle deformation regime transition, and the genetic link between these two contrasting episodes, if any, have been evaluated from statistical analysis of solid-state fabric and kinematic analysis of brittle fractures.

Three ductile deformation phases, D1, D2, and D3, and associated solid-state fabrics, i.e., S1, S2, and S3, are discernible at the mesoscopic scale. S1 fabric is gneissic in character and is only preserved in strain shadow regions. Elsewhere, S1 is transposed along the later S2 fabric, which is axial planar to fold on S1. Prevalence of high-temperature deformation conditions during D2 and D3 deformation stages is manifested by the presence of S2-parallel stromatic leucosomes and diatexite leucosome along dilatant S3 fabric, developed parallel to the axial planes of fold on S2. Significant simple shear component during D3 deformation is evidenced from the asymmetric nature of S2 folds, asymmetric porphyroclast tail and other shear sense markers. Eigen vector analysis reveals a change of maximum eigen vector, i.e., pole to the mean foliation, from NW-SE (D1: 311⁰/62⁰ NE) to N-S (D3: 187⁰/80⁰ W). The maximum eigen vector of D2 (125⁰/53⁰ SW), though similar in trend with D1, shows a reversal of dip direction. Fabric shape analysis reveals a progressive change from girdle to a strong clustered distribution of solid-state fabric from D1 to D3 deformation regime, suitably accounting for intense ductile shearing and transposition of earlier fabric during the D3 deformation stage.

Minor conjugate faults are ubiquitous at different locations along the AKSZ. Dihedral angle of ~60 or less for these faults suggests a shear or hybrid fracture origin, diagnostic of a compressive stress regime. Also, the observed slip of striations on slickensides suggests a consistent oblique reverse kinematics. Fault kinematic and paleo-stress analysis further reveals two distinct stress regimes with NW-SE and NE-SW directed maximum compressive stress (s1). Stress ratios for these faults imply a compressional to transpressional tectonic regime. Superposition of the slip tendency of NW–SE directed stress tensor over NE–SW directed stress tensor and vice-versa suggests that the NW-SE stress tensor precedes the NE-SW stress tensor during a progressive brittle deformation regime. Summarily, the cooling and exhumation and the switch over from ductile to brittle deformation regimes of the granulites took place under a compressive stress field developed during terrane accretion along the AKSZ. The brittle faults seemingly result from the relaxation of the orogenic far-field stress.

How to cite: Manilal Girija, A. and Bhadra, S.: Ductile to brittle tectonic evolution of the Achankovil Shear Zone, Southern Granulite Terrane – Constraints from statistical analysis of fabric and paleostress inversion, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20066, https://doi.org/10.5194/egusphere-egu26-20066, 2026.

EGU26-21372 | ECS | Posters virtual | VPS30

Dynamic Triggering and Effects of Crust Heterogeneities on Propagating Waves due to the 2025 Mw 7.7 Myanmar Earthquake 

Sneha Gupta, Vipul Silwal, and Sanjay Singh Bora

We investigate the heterogeneity of the Indian subcontinent using seismic recordings from the Mw 7.7 Myanmar earthquake that occurred on 28 March 2025. This event was recorded by broadband stations across India. These variations in waveforms at different stations highlight the influence of radiation pattern, crustal structure, wave-propagation paths, and local site conditions. Sedimentary basins, characterized by relatively soft sediments, are known to amplify seismic energy and modify ground motion characteristics, often resulting in enhanced shaking. Understanding these effects is essential for assessing seismic hazard.

We use time-series data from approximately 88 seismic broadband stations provided by the National Centre for Seismology (NCS), India. We apply frequency spectrum analysis, horizontal-to-vertical spectral ratio (HVSR) analysis, and surface wave dispersion analysis. The frequency spectrum helps identify frequency bands where seismic energy is amplified while HVSR analysis is used to estimate the site’s fundamental resonance frequency and the corresponding amplification factor. Surface wave dispersion analysis provides shear-wave velocity information, which is crucial for characterizing near-surface geological conditions.

Together, these analyses help us to understand the influence of local geological conditions at the receiver sites and contributes to a better analysis of regional seismic wave propagation and site-specific ground motion characteristics across the Indian subcontinent.

How to cite: Gupta, S., Silwal, V., and Bora, S. S.: Dynamic Triggering and Effects of Crust Heterogeneities on Propagating Waves due to the 2025 Mw 7.7 Myanmar Earthquake, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21372, https://doi.org/10.5194/egusphere-egu26-21372, 2026.

EGU26-21385 | ECS | Posters virtual | VPS30

Constraining Late Pleistocene to Holocene seismic fault activity in NE Iberia: The value of integrating complementary techniques in a low-strain region 

Marc Ollé-López, Julián García-Mayordomo, John Gallego-Montoya, Júlia Molins-Vigatà, Fabian Bellmunt, Anna Gabàs, Juvenal Andrés, Albert Macau, Altug Hasözbek, Anna Martí, Paula Figueiredo, Ángel Rodés, David García, María Ortuño, and Eulàlia Masana

The northeastern margin of the Iberian Peninsula, extending from the Vallès-Penedès Graben to the Valencia Depression, constitutes a passive margin related to the opening of the Valencia Trough during the Neogene. It comprises a series of extensive basins bounded by several mountain ranges, where numerous NNE–SSW-oriented normal faults are present, commonly associated with mountain fronts. Previous studies show that some of these faults, such as the El Camp fault, remain active, although at very low slip rates, as low as 0.02 m/kyr for Late Pleistocene.
Recent analyses of high-resolution Digital Elevation Models (DEMs) have revealed several additional morphological escarpments crosscutting different Quaternary alluvial fan systems across the region. These scarps, found from the Sant Jordi Plain to the La Salzadella Basin, share the same orientation as the Neogene faults, suggesting a common tectonic origin. They are discontinuous, arranged in a right-stepped pattern, and locally display vertical offsets of up to 8 m. Furthermore, several geomorphic features indicate recent tectonic activity, including aligned fissures within the fans and entrenched channels developed on the upthrown block that fade out after crossing the escarpments. Each family of escarpments exceeds 10 km in length, with important implications for the seismic hazard of the region.
Geophysical surveys (ERT, GPR, SRT, HVSR, and MT), validated with borehole data, confirm the presence of faults beneath each analysed escarpment system. At the Vinaixarop escarpment, for instance, ERT profiles revealed a steeply dipping discontinuity plane with a vertical offset of approximately 40 m affecting upper Pliocene sediments.
The faulted alluvial fans are interpreted as Lower to Middle Pleistocene in age and are mainly composed of carbonate gravels. Paleoseismological trenches excavated at four sites (L’Ampolla, Vinaixarop, and two at Sant Rafael del Riu) on different scarps revealed consistent evidence of late Quaternary faulting, such as ruptured strata. Additionally, ground-based hyperspectral cameras (400–1700 nm) were deployed on trench walls as an ancillary tool to map faulted
stratigraphic layers and to detect subtle coseismic deformation. As sedimentation on the fans ceased by the Middle Pleistocene, subsequent activity has been primarily recorded through the deformation of pedogenic features (calcretes), commonly found in the study area. To constrain the timing of this activity, U–Th dating was performed on fault-related carbonates and deformed calcretes. Preliminary results indicate that tectonic activity along these faults persisted at least until the Late Pleistocene. However, a deformed colluvial wedge and the presence of open fissures observed on trench walls suggest Holocene activity.
Additionally, three cosmonuclide depth-profiles were sampled to date displaced geomorphic surfaces, and hence estimating the long-term slip rates of the faults. Ongoing analyses aim to demonstrate Holocene seismic activity and to further characterize paleoearthquakes and their seismic parameters.
In summary, studies of active tectonics in regions of very low strain are inherently challenging, especially when recent sedimentation is scarce and pedogenic processes are intense. Nevertheless, this work highlights that integrating multiple complementary techniques is the most effective approach to address such settings.

How to cite: Ollé-López, M., García-Mayordomo, J., Gallego-Montoya, J., Molins-Vigatà, J., Bellmunt, F., Gabàs, A., Andrés, J., Macau, A., Hasözbek, A., Martí, A., Figueiredo, P., Rodés, Á., García, D., Ortuño, M., and Masana, E.: Constraining Late Pleistocene to Holocene seismic fault activity in NE Iberia: The value of integrating complementary techniques in a low-strain region, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21385, https://doi.org/10.5194/egusphere-egu26-21385, 2026.

EMRP1 – Rock and Mineral Physics

EGU26-159 | ECS | Posters on site | EMRP1.1

Petrographic, physico-mechanical, and geochemical characteristics of Eocene sedimentary rocks from the Tbilisi Area (Georgia) 

Anzor Giorgadze, Benjamin Busch, Yonghui Chen, Chaojie Cheng, Victor Alania, Levan Gorgidze, and Onise Enukidze

The Tbilisi Area is located within the eastern segment of the Achara-Trialeti fold-and-thrust belt, which is itself a part of the Kura foreland basin system. The region is characterized by an active convergent tectonic regime resulting from the ongoing collision between the Eurasian and Arabian plates. The convergence has induced extensive deformation features, including large-scale folding, faulting, and uplift, which have influenced the stratigraphy and lithological compositions of the Eocene sedimentary rocks of the study area.

A detailed, interdisciplinary study of these Eocene sedimentary rocks was implemented, integrating petrographic, geochemical, geomechanical, and petrophysical analyses to comprehensively understand physico-mechanical properties, and their interrelation. For this purpose, samples taken from the field were analysed at the Institute of Applied Geosciences, KIT. Petrographic examinations reveal a heterogeneous lithological assemblage comprising predominantly fine-grained clay mineral matrix-rich arkosic wackes, lithic wackes, arkosic arenites, and lithic arenites often containing foraminifera and glauconite, implying marine deposition. Geochemical analyses indicate the most prominent elements of the rocks are Si, Al, and Ca. Their content ranges 23.2-29.6%, 7.1-10.1%, 1.7-11.6%, respectively.

The rocks exhibit notably low permeability, generally in the range of 10-4 to 3*10-1 millidarcies (mD), with permeability strongly dependent on porosity metrics (ranging from 1.1% to 10.3%). This low permeability is primarily controlled by clay matrix content and to a lesser extent on cementation processes. The heterogeneity and complexity of these formations are further confirmed by the wide range of uniaxial compressive strength (UCS), from 36.9 MPa to 208.8 MPa, reflecting variations in lithology, degree of cementation, and diagenetic modifications across different sections.

This work presents an initial effort to showcase the diverse rock properties from the Tbilisi Area, as the Eocene sedimentary rocks show distinct lithological heterogeneity and complex mineralogical and petrophysical characteristics, strongly influenced by their depositional and tectonic history with implications for engineering utilization of the lithologies.

Acknowledgement: This work was supported by the Joint Rustaveli-DAAD fellowship programme, 2025. We thankfully acknowledge assistance in the lab by Martin von Dollen (KIT).

How to cite: Giorgadze, A., Busch, B., Chen, Y., Cheng, C., Alania, V., Gorgidze, L., and Enukidze, O.: Petrographic, physico-mechanical, and geochemical characteristics of Eocene sedimentary rocks from the Tbilisi Area (Georgia), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-159, https://doi.org/10.5194/egusphere-egu26-159, 2026.

Abstract

To identify and characterize reservoir and non-reservoir intervals across multiple formations, this paper examines comprehensive petrophysical evaluation and scattered cross-plot analysis using well-log data from Well 32-2-1 in the Smeaheia area of the Norwegian North Sea. The main objective of this study is to delineate lithology variations, detect fluid-bearing zones, and evaluate the key geological and petrophysical factors that control reservoir quality within a heterogeneous sandstone-shale succession.

A suite of well logs including gamma ray, resistivity, density, neutron porosity, and sonic measurements was thoroughly interpreted to identify lithological transitions and potential hydrocarbon-bearing intervals. Cross-plotting techniques were employed to analyze relationships between critical log parameters such as RHOB-NEU, GR-density, and neutron-density separation etc. These crossplots facilitated the differentiation of claystone, shaly-sand, clean sandstone, cemented sandstone, and coal units, while also revealing variations in porosity, mineral composition, and clay content across the well.

The integrated petrophysical analysis highlighted significant vertical heterogeneity, ranging from clean quartz-rich sandstones to shaly sands, claystone-dominated sections, calcite-cemented sands, and thin coal streaks. High gamma-ray, moderate density, and elevated neutron porosity responses delineate clay-rich zones where bound water inflates apparent porosity. Shaly-sand units are identified through intermediate clustering in RHOB-NEU and GR-density crossplots, reflecting mixed mineralogy and moderate effective porosity. Clean sandstone intervals, recognized by low GR and low NEU signatures, exhibit variable reservoir quality controlled by burial compaction and cementation intensity. Zones showing lower-than-expected density and reduced sonic velocity indicate undercompaction and suggest localized overpressure conditions.

Overall, the results of this cross-plot-driven petrophysical evaluation provide new insights into the distribution of porosity, clay volume, compaction state, and lithofacies variability throughout the stratigraphic interval. The interpretation enhances the understanding of reservoir and non-reservoir facies and improves the identification of intervals with potential hydrocarbon significance. The findings of this study contribute to more reliable reservoir characterization and support improved exploration and development strategies within the complex sandstone systems of the Norwegian North Sea.

 

Keywords:  Rock Physics, Petrophysics, Reservoir zone, Cross-Plot, Smeaheia Region.

How to cite: Rani, P. and Yadav, A.: Cross-Plot-Driven Petrophysical and Rock Physics Characterization of Reservoir and Non-Reservoir Zones in the Smeaheia Area, Norwegian North Sea, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-688, https://doi.org/10.5194/egusphere-egu26-688, 2026.

EGU26-1712 | ECS | Posters on site | EMRP1.1

Nonlinear viscoelastic constitutive relation for rocks under micro-strain dynamic loading 

Han Bai, Xuan Feng, Michael Fehler, Stephen Brown, and Götz Bokelmann

Rocks exhibit pronounced nonlinear viscoelastic behavior such as modulus softening and loading–unloading hysteresis, even under micro-strain dynamic loading. However, classical nonlinear elastic constitutive models based on higher-order expansions of Hooke’s law show limitations in capturing these nonlinear viscoelastic features. To address this, we extend the classical nonlinear elastic framework by incorporating strain-rate terms and formulate a nonlinear viscoelastic constitutive relation in which nonlinear elastic and viscoelastic parameters jointly describe modulus softening, dynamic response, and hysteresis loops. We use a copropagating acousto-elastic testing system to acquire time series of elastic modulus variation ΔM/E and the corresponding hysteresis loops for Crab Orchard sandstone at five dynamic strain levels. We then invert these data to estimate model parameters and test the constitutive relation. The model reproduces the main nonlinear viscoelastic features observed at all strain levels and, compared with two classical nonlinear elastic models without viscoelastic terms, better captures the phase information in the ΔM/E time series and the geometry of the hysteresis loops. The proposed nonlinear viscoelastic constitutive relation provides a practical way to constrain micro-strain nonlinear viscoelastic parameters of rocks in the laboratory and offers a basis for linking laboratory measurements with field relative velocity changes monitoring to study stiffness evolution during processes such as hydrological loading and fault slow slip.

How to cite: Bai, H., Feng, X., Fehler, M., Brown, S., and Bokelmann, G.: Nonlinear viscoelastic constitutive relation for rocks under micro-strain dynamic loading, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1712, https://doi.org/10.5194/egusphere-egu26-1712, 2026.

Characterizing and predicting reservoir heterogeneity is essential for efficient hydrocarbon production. In this study, multifractal theory is employed, using both numerical and experimental data, to quantitatively describe the pore structure heterogeneity of a Lower Cretaceous limestone reservoir from the United Arab Emirates. Fractal dimensions derived from three-dimensional digital images show a strong correlation with high-pressure mercury injection (HPMI) measurements (R² = 0.69). Furthermore, both experimental and numerical fractal dimensions correlate well with HPMI-derived porosity. Multifractal parameters—including the non-uniformity degree of the pore structure (Δα), the asymmetry in the vertical axis (Δf(α)), the concentration of the pore size distribution (α₀), and the asymmetry in the horizontal axis (Rd)—calculated from digital and experimental data, are consistently correlated and demonstrate a robust ability to quantify sample heterogeneity. The ranges of these digital and experimental multifractal parameters provide an effective basis for distinguishing between homogeneous and heterogeneous samples.

How to cite: Jouini, M. and Bouchaala, F.: Multifractal Parameters as Indicators of Pore Structure Heterogeneity in a Lower Cretaceous Limestone Reservoir (UAE), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2023, https://doi.org/10.5194/egusphere-egu26-2023, 2026.

EGU26-3035 | Posters on site | EMRP1.1

The impact of consolidants on the properties of intact and damaged porous limestones 

Patrick Baud, Perrine Schloegel, Fabrice Surma, Thierry Reuschle, and Michael Heap

Natural stones used in most buildings undergo degradation due to their exposure to outdoor environments, particularly to sometimes extreme variations in temperature and humidity conditions. In historical buildings, consolidants are often used to restore the strength of the damaged building materials and prevent further deterioration. The most commonly used consolidant in this context is ethyl silicate but it is incompatible with salt-contaminated stone. A salt-compatible alternative, lithium silicate, has been developed but remains rarely used. This is partly due to the limited number of available scientific studies and the difficulty of detecting lithium using conventional analytical methods. The aim of this study was to compare the effectiveness of these consolidants on two porous limestones subjected to thermal and mechanical stresses. Saint-Maximin and Leitha limestones were selected for this study because both rocks were widely used as building stones, in France and Austria, respectively. Cylindrical samples of 40 mm in length and 20 mm in diameter were prepared from large blocks. The average porosities of our Saint-Maximin and Leitha limestones were 38% and 41%, respectively. The permeability of both limestones was greater than 1 Darcy. Three groups of samples were tested: intact samples, samples thermally treated up to 400°C and samples deformed uniaxially to the peak stress. Consolidants were introduced in these samples through imbibition experiments that lasted a minimum of 48 h. Within the limestones, the consolidants underwent hydrolysis and condensation reactions to first form a gel on the pore surface. This gel progressively polymerized to form a thin solid layer on the pore surface. Treated samples were typically left to cure in a dry environment for at least a month. Minor variations of the porosity and permeability were observed in all the consolidated samples. The Uniaxal Compressive Stress (UCS) of the intact samples predictably increased by a factor of two for both rocks and both consolidants. After thermal treatment up to 400°C, the UCS of samples of Saint-Maximin and Leitha typically decreased by about 25% due to the thermal expansion of the grains and thermal microcracking. We found that consolidation with ethyl silicate erased this weakening effect. For lithium silicate, the samples also recovered part of their strength, but the effect was less pronounced. When damage was introduced into the rocks through uniaxial compression, ethyl silicate produced a more significant strengthening effect than lithium silicate. In the context of cultural heritage conservation, it is essential that consolidated stones present petrophysical properties similar to the original material in order to prevent further mechanical alterations. Both products exhibit a consolidating effect, but stones consolidated with lithium silicate display properties closer to those of the original rock.

How to cite: Baud, P., Schloegel, P., Surma, F., Reuschle, T., and Heap, M.: The impact of consolidants on the properties of intact and damaged porous limestones, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3035, https://doi.org/10.5194/egusphere-egu26-3035, 2026.

Elastic and electrical properties of a fluid-bearing rock are strongly affected by cracks. Effective elastic compliance of a rock is determined by number density and compliance of cracks. When cracks form an interconnected network, effective electrical conductance is determined by number density and conductance of cracks. Cracks have rough surfaces and asperities on them come into contact under pressure. Elastic compliance and electrical conductance of a crack decrease with its closure to govern changes in elastic and electrical properties with pressure. Though surface topography of cracks is a key to understanding physical properties under pressure, it is still difficult to investigate. We thus conduct numerical experiments of crack closure to understand changes in elastic and electrical properties with pressure. For simplicity, a 2D 50×50 square lattice is used to model a fluid-filled crack. The initial aperture of cells has a Gaussian distribution and is randomly given. For a closure of aperture, the required stress is calculated through Hertzian contact theory and electrical conductance of the lattice is calculated with the finite difference method. The lattice is electrically conductive when more than 50% of cells are open. When more than 70% of cells are open, the conductance is insensitive to the distribution of apertures. The elastic compliance is also calculated as a function of aperture closure. Both elastic and electrical properties are thus obtained as a function of confining pressure and compared with measured elastic wave velocity and electrical conductivity reported in Watanabe et al. (2019, 2024).

How to cite: Watanabe, T.: Numerical experiments of crack closure and its influence on elastic and electrical properties, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3760, https://doi.org/10.5194/egusphere-egu26-3760, 2026.

EGU26-4113 | Posters on site | EMRP1.1

Contrasting seismic velocity and compaction of marine calcareous oozes and volcaniclastic deposits 

Michael Manga, Vashan Wright, Tyler Cadena, Isabelle Susman, Carla Escogido, Sarah Ward, Liam Kelly, Kristen Fauria, Iona McIntosh, Jonas Preine, Masako Tominaga, Paraskevi Nomikou, Tim Druitt, Steffen Kutterolf, Thomas Ronge, Christian Hübscher, Jens Karstens, and Yuzuru Yamamoto and the IODP Expedition 398 Scientists

We compare and contrast physical properties (density, P-wave velocity) of volcaniclastic sediments with other uncemented marine sediments. We study cores collected by International Ocean Discovery Program (IODP) Expedition 398, which recovered more than 2200 m of volcaniclastic deposits from 12 sites and 28 holes from Santorini Caldera, Greece, and the surrounding rift basins in the South Aegean Volcanic Arc. The grain density (mass of solids divided by their volume, including any isolated vesicles) of volcaniclastic deposits is typically lower than that of volcanic glass and crystals and is sometimes less than 2 g/cm3, indicating the preservation of isolated gas-filled vesicles in erupted and then deposited materials. To complement bulk measurements, we also measured the total and isolated porosity in individual lapilli-sized volcanic clasts from four different volcanic deposits. We use xray computed tomography to image isolated pore space. Collectively, these measurements confirm that volcaniclastic sediments can preserve vesicle textures and isolated porosity for hundreds of thousands of years and at depths >500 m below sea-level and > 100 m below the seafloor

 

Volcaniclastic deposits typically have higher P-wave velocities but lower bulk densities than oozes and other marine sediments. In volcaniclastic deposits, lapilli have higher P-wave velocities and lower bulk density than ash, the opposite trend of most sediment in which higher density is correlated with higher seismic velocity. We use granular physics models to show that the higher volcaniclastic P-wave velocity originates from two effects: 1) lower pore volume outside clasts that increases elastic moduli and P-wave velocity and 2) isolated gas vesicles in volcanic clasts that lower bulk density with proportionally less effect on elastic modulii. In volcaniclastic sediments there is relatively little change in physical properties to depths of several hundred meters below the seafloor, which we attribute to rough grain surfaces and lower intergranular (external) porosities that resist compaction and the decrease of intergranular pore space relative to background marine sediment.  These trends lead to distinctive signatures of volcaniclastic sediments in reflection seismic images.

 

How to cite: Manga, M., Wright, V., Cadena, T., Susman, I., Escogido, C., Ward, S., Kelly, L., Fauria, K., McIntosh, I., Preine, J., Tominaga, M., Nomikou, P., Druitt, T., Kutterolf, S., Ronge, T., Hübscher, C., Karstens, J., and Yamamoto, Y. and the IODP Expedition 398 Scientists: Contrasting seismic velocity and compaction of marine calcareous oozes and volcaniclastic deposits, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4113, https://doi.org/10.5194/egusphere-egu26-4113, 2026.

EGU26-4727 | ECS | Orals | EMRP1.1

Rock physics model for patchy saturated porous media under in-situ stress 

Jiayun Li, Zhaoyun Zong, Fubin Chen, and Xuan Zheng

In situ stress and wave-induced fluid flow (WIFF) jointly influence the velocities of waves propagating through the formations. However, for partially saturated porous media commonly encountered in the subsurface, the stress- and frequency-dependent characteristics of wave velocity dispersion and attenuation are not yet fully understood. To address this, we propose a new poro-acoustoelasticity model to characterize wave velocities in patchy-saturated porous media under in-situ stress. This model simultaneously accounts for macroscopic global flow arising from wave-induced relative motion between the pore fluid and the solid frame, mesoscopic WIFF associated with patchy fluid saturation, and microscopic squirt flow induced by fluid pressure gradients between pores and cracks. Furthermore, by considering the influence of effective stress on the pore structure, the nonlinear deformation of cracks is incorporated into our rock physics model, thereby extending its stress applicability. The modelling results indicate that two compressional waves (fast P- and slow P-waves) and a shear wave (S-wave) coexist. As the effective stress increases, the velocities of the fast P- and S-wave increase, accompanied by reductions in dispersion and attenuation, which can be attributed to crack closure. In addition, with increasing frequency, the fast P-wave velocity exhibits three successive attenuation peaks, corresponding to the effects of WIFF at meso-, micro-, and macro-scales. In contrast, the slow P-wave velocity appears only at higher frequencies, and its variation is more significantly influenced by water saturation than by effective stress. The validity of the proposed model is demonstrated through comparison with previously published experimental data. Furthermore, our model is used to establish a rock-physics approach to estimate the wave velocities with the well-logging data. The predicted results agree well with the logging measured data, further confirming the feasibility of our approach. Our study and results provide a useful tool for hydrocarbon exploration, CO2 storage monitoring, and hydrogeology.

How to cite: Li, J., Zong, Z., Chen, F., and Zheng, X.: Rock physics model for patchy saturated porous media under in-situ stress, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4727, https://doi.org/10.5194/egusphere-egu26-4727, 2026.

    The gravel deposit, widely distributed in Taichung City, central Taiwan, is a composite material in which gravels and cobbles are embedded within a fine-grained soil matrix. Due to the presence of large particles ranging from 100 mm to 300 mm, the characterization of shear strength commonly relies on large-scale direct shear tests or triaxial tests. In practice, however, these measurements are costly and difficult to perform in sufficient numbers to represent the high variability of mechanical properties at the site. To address this limitation, this study proposes an integrated framework that incorporates the hardness value of the matrix, obtained from the Yamanaka soil hardness tester, and the geometric features of gravels into Discrete Element Method (DEM) simulations to estimate the shear strength of the gravel deposit.

    Specifically, three-dimensional DEM simulations were conducted using EDEM, employing the Hertz-Mindlin contact model coupled with the Bonded Particle Model (Bonding V2) to replicate a full-scale direct shear test. The gravel deposit was discretized into matrix (< 4.75 mm) and gravel (> 4.75 mm) fractions based on the field investigation results. To represent the geometric heterogeneity, image analysis was employed to characterize the gravel fraction and extract morphological parameters for the simulation. Under this classification, distinct approaches were adopted for the micro-parameters. Contact parameters were specified for each fraction, while bonding parameters for all interaction types (Matrix-Matrix, Matrix-Gravel, and Gravel-Gravel) were governed by the matrix properties. To determine the appropriate bonding and contact parameters specific to the matrix fraction, the Yamanaka soil hardness tester was utilized to bridge the gap between field conditions and numerical simulations. By employing Response Surface Methodology (RSM), a quantitative relationship between micro-parameters and penetration depths was established to identify the parameters from the field data. Subsequently, the calibrated micro-parameters corresponding to the target in-situ penetration depth were assigned to the composite model for full-scale direct shear test simulations to evaluate the shear strength. Preliminary verification confirms the feasibility of the penetration test simulation in EDEM. Furthermore, complementary uniaxial compression tests demonstrate that the calibrated bonding parameters correspond to realistic physical properties, thereby ensuring the reliability of the shear strength estimation in the full-scale DEM simulations.

 

How to cite: Liu, P.-C. and Chang, K.-T.: Estimating the Mechanical Properties of Gravel Deposits by Integrating Field Investigation and DEM Simulation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4766, https://doi.org/10.5194/egusphere-egu26-4766, 2026.

EGU26-7308 | ECS | Orals | EMRP1.1

Controlling factors of petrophysical and sedimentary heterogeneities in Paleogene rocks beneath Paris, France 

Charlie Marconnet, Cédric Bailly, Justine Briais, Jean-Baptiste Regnet, Simon Andrieu, Eric Lasseur, and Benjamin Brigaud

The Paleogene sedimentary series of the Paris Basin, characterized by mixed carbonate and siliciclastic deposits in continental and marine environments, exhibit significant lithological, facies, and diagenetic heterogeneities. However, the lack of data and conceptual frameworks linking petrophysical properties to geological knowledge of these sedimentary series remains a major limitation for predicting physical properties across different scales. Understanding and predicting reservoir heterogeneities is essential for addressing major societal challenges, such as subsurface planning and geothermal energy development in the Île-de-France region. To tackle this issue, a multi-scale study is conducted, integrating sedimentary geology and petrophysical analyses of the Paleogene series. The study focuses on key areas of the Paris Basin, defined by the alignment of the Grand Paris Express (GPE) project, a 200 km network of new metropolitan lines around Paris. These areas are ideal to lead to a very high spatial resolution characterization of the sedimentary system, thanks to the availability of an exceptionally dense dataset of core drillings.

The analysis of cores from 15 boreholes and gamma-ray logs from 34 additional boreholes allowed the identification of twenty-two facies grouped into seven facies associations, corresponding to seven depositional environments ranging from open marine environments to palustrine settings. Based on these observations, twelve transgressive–regressive cycles spanning the Danian to the Rupelian were identified and correlated along two multi-kilometer transects (≈20 km).

Petrophysical measurements performed on 633 samples reveal a strong heterogeneity within the studied Paleogene successions. For instance, palustrine limestone facies affected by intense recrystallization and silicification display relatively uniform P-wave velocities (4.1–6 km s⁻¹) and porosities (1.5%–12%). In contrast, marine limestones exhibit a wide range of P-wave velocities (0.9–5.6 km s⁻¹), partly related to facies variability and primarily controlled by porosity (5–46%), with decreasing velocities at increasing porosity. This parameter is mainly governed by the abundance and nature of diagenetic cements, with mosaic calcite cements (drusy, granular, blocky) leading to a stronger porosity reduction than isopachous cementation, while depositional facies exert a secondary control (e.g. Miliolid grainstone vs Bioclastic floatstone). Additional controls contributing to the petrophysical heterogeneity of marine limestone facies include pore spatial distribution and connectivity, pore size distribution, and pore type. Pore spatial organization exerts a first-order control on acoustic velocities and porosity: uniformly distributed and well-connected pore networks are associated with low P-wave velocities and high porosities, whereas patchy pore distributions lead to higher velocities and reduced porosity. Pore size also influences petrophysical properties, with macroporosity (>62 µm) generally associated with relatively high P-wave velocities and low porosities, while meso-microporosity (<62 µm) does not show a clear relationship with either parameter. Pore type also plays a significant role, as interparticle porosity is associated with low velocities and high porosities, in contrast to intraparticle, moldic, and vuggy porosities, which are characterized by higher velocities and lower porosities.

Although locally homogeneous from a petrophysical perspective, these sedimentary series display strong heterogeneities governed by multiple geological controls, emphasizing the key role of petrophysical characterization in reservoir prediction.

How to cite: Marconnet, C., Bailly, C., Briais, J., Regnet, J.-B., Andrieu, S., Lasseur, E., and Brigaud, B.: Controlling factors of petrophysical and sedimentary heterogeneities in Paleogene rocks beneath Paris, France, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7308, https://doi.org/10.5194/egusphere-egu26-7308, 2026.

EGU26-8295 | ECS | Orals | EMRP1.1

Exploring seismic velocity transients using in-situ acoustic monitoring and synchrotron-based X-ray tomography in triaxial dynamic loading experiments 

Xun Li, Michael Chandler, Alexis Cartwright-Taylor, Damien Freitas, Maria-Daphne Mangriotis, Birhanmeskel Woldemichael, Alexander Liptak, Robert Atwood, Mark Chapman, Florian Fusseis, Ian Butler, Andrew Curtis, and Ian Main

Seismic velocity at the near surface drops during ground motions due to remote earthquakes and can recover afterwards over decades. In the laboratory, seismic velocity of rock samples decreases after dynamic deformations (e.g., shaking) and gradually recovers towards the original level. These observations at different scales are referred to as slow dynamics in granular materials (e.g., rocks and concrete), but the underlying mechanisms remain debated.

We explore the physics behind seismic velocity transients during and after dynamic deformations using Stór Mjölnir — a triaxial pressure loading apparatus featuring two piezoelectric transducers mounted in the top and bottom pistons and an X-ray transparent aluminium pressure vessel that houses a cylindrical core sample of Clashach sandstone (10 mm in diameter and 25 mm in length).

We present the mechanical, acoustic, and X-ray microtomography results of two triaxial loading experiments, conducted at room temperature with a confining pressure of 20 MPa and a pore fluid pressure of 5 MPa. Both experiments involve first increasing the ram pressure at a constant strain rate of 1x10-5 s-1 until the onset of sample yielding, indicated by a deviation from the linear stress–strain curve. In the first experiment, we further hold the ram pressure constant and then abruptly reduce the pressure by 30 MPa before rapidly returning the pressure to the previous hold level; this perturbation is repeated for 32 cycles until catastrophic failure of the rock sample. In the second experiment, we apply the same cyclic loading protocol after sample yielding, except for the abrupt pressure drop of 150 MPa; the sample survives only two loading cycles before catastrophic failure. These cyclic loading protocols are designed to induce transient seismic velocity responses, which are monitored by active acoustic surveys acquired every 8 s and in-situ 3D X-ray tomography synthesised every 6 min at the beamline I12-JEEP, Diamond Light Source (Oxfordshire, UK).  

We observe nearly linear relationships between the small stress perturbations (30 MPa) and corresponding seismic velocity changes, indicating minimal slow dynamics in the rock sample. In contrast, large stress perturbations (150 MPa) cause nonlinear velocity changes, although the recovery time scale is limited by the small size of the experimental sample. The time-resolved 3D X-ray volumes from both experiments show no resolvable transient structural changes in the rock samples, despite ongoing microfracture accumulation and pore enlargement driven by background creep until catastrophic failure. These results demonstrate that active seismic waves can detect nonlinear velocity transients in triaxial loading experiments, which likely originate from microstructures (e.g., grain contacts) below the X-ray imaging resolution (voxel edge length ~ 7.9 µm). These experiments also motivate further study on seismic velocity transients using our next-generation experimental apparatus that accommodates larger samples (18 mm in diameter and 45 mm in length) and six acoustic transducers. Ultimately, we aim to assess seismic velocity transients as a proxy for rocks’ susceptibility to small stress perturbations, which could provide a method to map the proximity to catastrophic failure and hence help mitigate induced seismicity associated with hydraulic fracturing.

How to cite: Li, X., Chandler, M., Cartwright-Taylor, A., Freitas, D., Mangriotis, M.-D., Woldemichael, B., Liptak, A., Atwood, R., Chapman, M., Fusseis, F., Butler, I., Curtis, A., and Main, I.: Exploring seismic velocity transients using in-situ acoustic monitoring and synchrotron-based X-ray tomography in triaxial dynamic loading experiments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8295, https://doi.org/10.5194/egusphere-egu26-8295, 2026.

EGU26-8989 | ECS | Posters on site | EMRP1.1

Frequency-Dependent Effective Electrical Properties of Suboptimal Rock Samples through Digital Rock Physics 

Nils Kerkmann, Mirko Siegert, Claudia Finger, Alexis Shakas, and Erik H. Saenger

Geothermal exploration drilling plays a crucial role in advancing the energy transition. To make the prospecting process more economical and time-efficient, the EU-funded GeoHEAT project has set the goal of developing methods that allow for obtaining the maximum amount of information about the subsurface with as little expense as possible. The project includes the development of a ground-penetrating radar (GPR) that can be used during borehole logging at elevated ambient temperatures. For the accurate interpretation of the GPR data, as well as for estimating the porosity and water content of the rocks surrounding the borehole, properties such as permittivity and electrical conductivity of these rocks are required. Here, we want to present the current progress of our research, which aims to determine the aforementioned characteristic properties using digital rock physics (DRP). Moving away from standardized cylindrical samples and using irregularly shaped by-products of the drilling process, known as drill cuttings, we can provide a more comprehensive understanding of the subsurface, thereby improving the characterization of potential geothermal reservoirs.

Core sampling during exploration drilling is costly and time-consuming, as it interrupts the operation. In addition, cores are often taken from only a few sections in order to keep the added costs low. However, these samples are necessary for laboratory testing, as sufficiently large and smooth contact surfaces must be available to ensure that the respective measurement devices deliver accurate results. No such requirements exist in DRP, as simulations are performed at the pore scale and therefore very small samples without flat surfaces, such as irregular drill cuttings, can be used.

The DRP workflow consists of three main steps. First, high-resolution computed tomography scans are taken of a small sample. These are then processed into a digital twin using segmentation, where the individual phases, such as minerals or pores, are distinguished from one another so that specific properties can later be assigned to them in this location-dependent volume. In combination with our finite volume method code, which solves a stationary potential equation, this digital model can be used to simulate the desired effective properties.

In previous studies, an early implementation of our code demonstrated reliable results for frequencies greater than 1 MHz. By implementing preconditioners, we now simulate lower frequencies with highly accurate results where before the increase in polarization led to code instabilities. Additionally, we fully validated the code on comparative data, such as analytical solutions and laboratory measurements of a high-porosity sandstone and a low-porosity granite. In the future, we will investigate how changes during the creation and transport of drill cuttings influence the accuracy of the results, thereby contributing further to a more efficient approach to geothermal exploration.

How to cite: Kerkmann, N., Siegert, M., Finger, C., Shakas, A., and Saenger, E. H.: Frequency-Dependent Effective Electrical Properties of Suboptimal Rock Samples through Digital Rock Physics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8989, https://doi.org/10.5194/egusphere-egu26-8989, 2026.

EGU26-9096 | ECS | Orals | EMRP1.1

Elucidating Pore-Scale Mechanisms Governing the Saturation-Dependence of Complex Conductivity 

Siyuan Qiang, Xiaoqing Shi, and André Revil

Petrophysical models linking geophysical observables to subsurface hydraulic states are fundamental to the interpretation of hydrogeophysical data. For electrical methods, power-law formulations such as Archie’s law are commonly used to relate different components of complex conductivity to water saturation, with the associated saturation exponents in these power laws describing the saturation-dependent behavior of complex conductivity. However, due to the lack of the ability to directly visualize pore-scale fluid distributions for traditional laboratory or field investigations, the physical origin and variability of these saturation exponents remain poorly understood, which hinders reliable interpretation of geoelectrical data in dynamic or heterogeneous subsurface environments.

In this contribution, we present results from our recent studies that quantitatively investigate how pore-scale fluid and interface distribution govern the saturation dependence of complex conductivity. First, a dedicated milli-fluidic micromodel was developed to enable simultaneous spectral IP measurements and direct visualization of pore-scale fluid configurations during drainage and imbibition. By combining laboratory observations with finite-element and pore-network simulations, we demonstrate quantitatively that both the in-phase and quadrature saturation exponents are controlled by the rate of change of pore-water connectivity with saturation. In parallel, by extending Archie’s laws to interfacial polarization using fractal theories, we establish that surface and quadrature conductivity in fractal porous media follow power-law relationships with specific surface area, with the corresponding exponents linked to the pore-volume fractal dimension. Building on these results, we further explore a commonly observed yet poorly explained anomaly in IP measurements: the decrease of quadrature conductivity (or normalized chargeability) with increasing saturation during drying. Using desiccation experiments combined with pore-network modeling, we show that this anomalous behavior arises from a coupled mechanism involving the sequential drying of pores of different characteristic sizes and the persistence of thin water films on solid surfaces.

Together, these studies advance the petrophysical understanding of IP signatures by linking macroscopic electrical parameters to microscale fluid topology and interfacial processes. Our findings underscore the importance of incorporating pore-scale fluid connectivity and interfacial effects into petrophysical models, thereby improving the quantitative interpretation of geoelectrical data in hydrogeological, biogeochemical, and reservoir monitoring applications.

How to cite: Qiang, S., Shi, X., and Revil, A.: Elucidating Pore-Scale Mechanisms Governing the Saturation-Dependence of Complex Conductivity, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9096, https://doi.org/10.5194/egusphere-egu26-9096, 2026.

Resolving hydrogeologic conditions in fractured bedrock aquifers poses unique challenges due to heterogeneity attributed to variability in fracture network characteristics, where fractures, if open and connected, serve as primary pathways for water flow and contaminant transport. Bedrock mechanical properties influence fracture frequency and connectivity, and thereby hydrologic unit (HGU) boundaries and hydraulic conductivity variations. In such aquifers, HGU boundaries are often associated with zones of poor vertical fracture connectivity, caused by the termination of vertical joints at changes in rock mechanical properties associated with bedding. Understanding these properties and boundaries is essential for improved hydrogeologic conceptual site models relied on for science-based groundwater management and source protection.  

This study focuses on downhole data collected in one cored hole within a regionally significant dolostone aquifer in the City of Guelph, Ontario, Canada.  Full Waveform Sonic (FWS) low-frequency energy attenuation, combined with other advanced borehole geophysical and hydraulic datasets, is used to investigate the relationship between insitu fracture characteristics and hydraulic properties for 9 depth-discrete intervals.    

The literature reports that attenuation of the Stoneley wave’s low-frequency energy can be diagnostic of wave-induced fluid motion and viscous dissipation associated with hydraulically open fractures; however, quantitative borehole-scale estimations remain scarce. We compare low-frequency energy attenuation under continuous (slow logging speeds of 0.2-0.3 m/min) acquisition with other complementary high-resolution borehole datasets to assess the relationship between fractures’ hydraulic properties and energy attenuation. The other datasets include high-resolution temperature, Nuclear Magnetic Resonance (NMR), as well as depth-discrete transmissivity from straddle packer testing and hydraulic head profiles from numerous, temporarily deployed pressure transducers sealed behind flexible fabric borehole liners. By linking fracture hydraulic properties and energy attenuation, the study aims to improve distinguishing hydraulically active fractures during borehole characterization to better understand fracture controls on aquifer and aquitard unit boundaries and contaminant transport in fractured sedimentary rocks. 

How to cite: Dannak, H., Pehme, P., Munn, J. D., and Parker, B. L.: Quantification of Low-Frequency Stoneley Wave Energy Attenuation in a Carbonate Fractured Bedrock Aquifer: An Evaluation of Its Relationship with Fracture Hydraulic Properties  , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12242, https://doi.org/10.5194/egusphere-egu26-12242, 2026.

EGU26-13896 | ECS | Posters on site | EMRP1.1

Integrating the multi-scale elastic velocities for interpreting and predicting the Dogger carbonate geothermal reservoir 

He-Ming Wang, Cédric Bailly, Benjamin Brigaud, Aurélien Bordenave, Benoit Issautier, Joshua Pwavodi, Chapman Samuel, Jérôme Fortin, Claire Le Romancer, Rabah Ould braham, Virginie Hamm, Camille Maurel, Damien Bonte, Giovanni Sosio, and Alexandre Stopin

The Dogger geothermal reservoir of the Paris Basin is one of the most actively exploited carbonate aquifers in France and serves as a key target for sustainable district-heating systems. It consists mainly of Middle Jurassic carbonates deposited on a ramp, where sedimentary facies and diagenetic overprinting produce strong spatial heterogeneity. Understanding the heterogeneous petrophysical distributions is essential for predicting fluid circulation and designing subsequent geothermal operation plan. However, petrophysical interpretations derived from geophysical methods remain scale-dependent: laboratory acoustic measurements, well logs, and seismic data have different resolutions, making it challenging to reconcile acoustic signatures and to map heterogeneity consistently across scales.

To address these challenges, we conducted ultrasonic transmission experiments on core fragments taken from the SEIF-01 geothermal well in Melun area to determine Vp and Vs across key facies types. We further measured pressure-dependent Vp-Vs variations on cylindrical plugs, to better understand how the sedimentary microstructures and crack closure control the seismic velocity. Using seismic rock velocity models, we interpret the influence of pore shape (measured by pore aspect ratio) and fluid on the seismic velocity, to provide a quantitative link between micro-scale pore geometry and macroscopic elastic properties.

Finally, we will integrate the laboratory results with in-situ sonic logs and 2D seismic reflection data to bridge acoustic observations across scales. This multi-scale integration provides new insights into the internal heterogeneity of the Dogger reservoir and improves the interpretation of geophysical datasets for geothermal development. Our results highlight the potential of combining ultrasonic experiments, well logs, and seismic data, to better constrain reservoir properties and support more reliable geothermal resource assessment in heterogeneous carbonate systems.

How to cite: Wang, H.-M., Bailly, C., Brigaud, B., Bordenave, A., Issautier, B., Pwavodi, J., Samuel, C., Fortin, J., Le Romancer, C., Ould braham, R., Hamm, V., Maurel, C., Bonte, D., Sosio, G., and Stopin, A.: Integrating the multi-scale elastic velocities for interpreting and predicting the Dogger carbonate geothermal reservoir, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13896, https://doi.org/10.5194/egusphere-egu26-13896, 2026.

     The thermal conductivity and thermal diffusivity of minerals and rocks under high temperature and pressure can provide data supporting for historical simulation of geological processes, and they are also necessary parameters for establishing the thermal structure of deep layer under a stable state.

     Amphibolite is a crucial component of the continental crust and subduction zone. The physical properties of amphibolite are of great significance for understanding the physical structure of the continental crust and subduction zones. In this study, using a thermal properties testing platform on a hinged cubic press, the thermophysical properties of two types of amphibolite were studied at 0.5-1.5 GPa and 300-973 K by the transient plane heat source method. The experimental results show thermal conductivity and thermal diffusivity decrease with the increasing of temperature and increase with the increasing of pressure. The influence of temperature on these parameters is much greater than that of pressure. Under fixed pressure, the thermal conductivity can vary up to 15.1% with temperature changes, while the thermal diffusivity can vary up to 40.0%. Under fixed temperature, the influence of pressure on the thermal conductivity can reach up to 23.4% and the influence on the thermal diffusion coefficient can reach up to 15.7%. The experimental data were successfully fitted using empirical formulas. The thermal conductivity and thermal diffusivity of garnet amphibolite in this study is notably higher than those of amphibolite without garnet and those reported in previous studies, so it is believed that the presence of garnet significantly enhances the thermal conductivity of amphibolite.

     Combining high-temperature and high-pressure data from previous studies as well as this study and the parameters of the thermal lithosphere model, the thickness of the thermal lithosphere in different regions of the North China Craton under different surface heat flows was calculated. The results reveal that within a surface heat flow range of 50-80 mWm-2, the thermal lithosphere thickness of the Bohai Basin varies between 49.8 and 145.7 km, the thickness of the central orogenic varies belt between 53.3 and 201.5 km, and the thickness of the Ordos Basin varies between 54.4 and 231.2 km.

How to cite: Yi, L. and Ma, W.: Thermal properties of garnet-bearing amphibolite at high temperature and pressure and its impact on the thermal structure of the lithosphere, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15505, https://doi.org/10.5194/egusphere-egu26-15505, 2026.

CO2 geological storage is key to combat global warming. During the site screening process, impact of seismic activity on the storage site is required [1]. As the Japan islands located in the convergent zone of four tectonic plates and are known as one of the most earthquake-prone countries in the world, evaluating and predicting the impact of great earthquakes on reservoirs and cap rocks and disseminating this information to society is especially important issues in terms of gaining social acceptance at the project planning stage.

 The authors are developing an earthquake response analysis method for evaluating the stability of CO2 geological storage sites in advance in the event of a great earthquake, but the input physical parameters of the cap and storage rocks under in-situ stress condition are not enough obtained. 

As the most of Japanese candidate storage sites are at young sedimentary formations, we prepare specimens (height 100mm, diameter 50mm) from Early Pleistocene sandstone and mudstone block sampled from outcrops. Triaxial compression tests were conducted under confining pressures corresponding to the depths of CO2 storage sites. The loading rate was performed at strain rates of 180%/min, 100%/min, and 10%/min. For instance, when a mudstone specimen was loaded at an effective confining pressure of 14 MPa, a back pressure of 9 MPa, and a strain rate of 180%/min, the maximum strength (approximately 6 MPa) appeared near an axial strain of 1%, after which a gradual softening trend was observed. Distinct strain-softening characteristics were not observed in this experiment. The pore pressure reached its peak slightly earlier than the maximum strength. Although it decreased thereafter, a slight upward trend was observed despite the decrease in axial deviator stress.

   In this presentation, we will report the strength and pore pressure characteristics of rocks based on rock types and loading rates, and propose strength parameters effective for dynamic analysis.

 

[1] International Organization for Standardization,2026, ISO standard 27914; Carbon Dioxide Capture, Transportation and Geological Storage – Geological Storage.

How to cite: Horikawa, S., Takemura, T., and Kusunose, K.: High Pressure Triaxial Compression Test in Soft Sedimentary Rocks —Relationship Between Loading Rate and Strength-Deformation properties—, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15718, https://doi.org/10.5194/egusphere-egu26-15718, 2026.

EGU26-15788 | ECS | Orals | EMRP1.1

Stochastic reconstruction of 2D volcanic rock pore structure using Growing Neural Cellular Automata 

Francisco Miguel Lechuga Lagos and Sandra Vega Ruiz

Characterizing rock pore structure is crucial for geothermal energy extraction, hydrocarbon assessment, and carbon capture and storage. The pore structure is conventionally estimated from core samples and well-log data. However, 2D images derived from drill cuttings offer an abundant and cost-effective alternative to complement lab and log analysis. Digital Rock Physics, combined with Artificial Intelligence, has the potential to provide robust tools to generate representative digital rock models directly from these 2D images. Specifically, Growing Neural Cellular Automata (GNCA) offer a distinct advantage; they follow simple learned local update rules and are efficient for emulating complex systems and natural phenomena, such as the regeneration of biological patterns and self-organizing textures. Moreover, they demonstrate training stability and low computational resource demands. Therefore, we propose training GNCA on 2D images to stochastically reconstruct the pore structure of selected volcanic rock samples to demonstrate the feasibility of the method. 

GNCA treat reconstruction as an evolving morphogenetic process, growing the pore structure iteratively from a seed state. Their lightweight architecture enables efficient training on consumer-grade hardware by utilizing gradient accumulation to handle input resolutions useful for pore-scale analysis (≥3202 px). A key contribution of our work is the physically-informed hybrid loss function, Ltotal, designed to bridge the gap between perceptual texture and physical topology:

Ltotal = Wvgg Lvgg + λ (Wtpcf Ltpcf + Wvt Lvt + Wα Lα + Wpor Lpor),

where: Lvgg captures local perceptual texture, while the physical constraints include Ltpcf for spatial statistics via the two-point correlation function, Lvt to regulate specific surface area via Total Variation, Lα to constrain global pore aspect ratio using the Global Inertia Tensor, and Lpor for porosity compliance. The weights Wi balance individual loss contributions, while λ modulates the trade-off between perceptual quality and physical fidelity. 

This model was trained using micro-CT slices from distinct volcanic samples from the Los Humeros Geothermal Field, Mexico. For validation, we compare the stochastic reconstructions against randomly selected reference slices. We also evaluate the standard two-point correlation function S2(r) and the two-point cluster function C2(r) to assess the pore spatial distribution and topological connectivity, respectively. In addition, the morphological fidelity is assessed via non-cumulative Pore Size Distribution and Aspect Ratio Distribution histograms, ensuring that the model captures the shape diversity of volcanic vesiculation. Furthermore, we implement a spectral analysis using the indicator function's Fourier transform, χV(k), which demonstrates that GNCA reproduce power spectral density across spatial frequencies, from macro-structures to fine details. Finally, the trained model successfully generates complete stochastic slices that are statistically equivalent to the original images at a 95% confidence level. This demonstrates that GNCA are efficient for reconstructing the studied volcanic samples.

In conclusion, the proposed GNCA framework, constrained by a physically-informed hybrid loss function, constitutes a viable alternative for the stochastic reconstruction of complex pore topologies in 2D images, yielding high-fidelity results on the analyzed volcanic rock samples.

How to cite: Lechuga Lagos, F. M. and Vega Ruiz, S.: Stochastic reconstruction of 2D volcanic rock pore structure using Growing Neural Cellular Automata, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15788, https://doi.org/10.5194/egusphere-egu26-15788, 2026.

EGU26-15944 | ECS | Orals | EMRP1.1

Insights into Fault Roughness Throughout the Seismic Cycle of Laboratory Earthquakes  

Isabelle Lambert and Nicola Tisato

Earthquakes are produced by slip events along faults driven by the accumulation and release of elastic energy in the Earth’s crust. They are cyclic, and a broad spectrum of slip behaviors is observed along seismogenic faults. The irregular and chaotic nature of earthquakes makes it difficult to establish a predictive law. Furthermore, the constitutive behavior of active fault zones remains a subject of debate, particularly regarding the relative roles of static and dynamic energy controls during seismic events. Elastic energy accumulation in the crust leads to rupture nucleation, while rupture propagation and arrest are likely governed by the physical properties of the fault zone, which vary between events and evolve during slip. While numerous parameters have been proposed to influence these processes, we emphasize that fault geometry and fault–fault interactions represent fundamental controls on rupture behavior and the evolution of the seismic cycle. To better understand how the size and distribution of asperities along faults control the earthquake cycle, we conducted laboratory experiments on analog material samples with root-mean-square (RMS) roughness values ranging from 0.5 to 30 micrometers. We used the Energy-Controlled Rotary Shear (ECoR) apparatus to replicate the earthquake cycle in the laboratory. The ECOR allows for spontaneous nucleation of laboratory earthquakes at velocities, accelerations, displacements, and magnitudes comparable to those observed in natural earthquakes. In these experiments, we used a loading spring with an effective elastic constant and varied the sample-averaged normal stress. Across experiments, we observe a range of slip behaviors, from stick–slip to steady creep, over the lifetime of the laboratory fault. We hypothesize that the size and distribution of asperities along the fault control the style of fault slip. Furthermore, over the course of the seismic cycle and in the presence of frictional weakening, we propose that the power density, another aspect that we will explore in the future, and the critical nucleation size control the magnitude of earthquakes.

How to cite: Lambert, I. and Tisato, N.: Insights into Fault Roughness Throughout the Seismic Cycle of Laboratory Earthquakes , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15944, https://doi.org/10.5194/egusphere-egu26-15944, 2026.

Across the central and western expanses of China, where soft rock formations dominate the geological landscape, arch bridges have long reigned supreme as the preferred structural choice. Their foundations, ingeniously engineered with a stepped-block configuration, boast exceptional overall rigidity—striking a masterful balance between structural integrity and economic efficiency by curbing infrastructure costs without compromising on deformation resistance. Drawing upon the foundational engineering of the Lantian Yangtze River Five Bridges, this study embarks on a profound investigation into the load-bearing behavior of stepped block foundations embedded within soft rock strata. It introduces a refined rigid-flexible judgment criterion and unveils an advanced, standard-anchored Optimization Specification C Method for stress-displacement analysis—a paradigm shift in computational precision. A novel analytical formula for the local shear failure angle is derived, shedding light on the underlying mechanics of shear collapse, while the verification framework for foundation deformation characteristics is meticulously enhanced. The culmination of this research is a comprehensive, high-fidelity bearing performance analysis system, exquisitely tailored for practical engineering application. Key findings reveal that both the rigid-flexible classification and the Optimization Specification C Method are eminently suited for assessing the bearing capacity of stepped arch foundations in soft rock environments, with design protocols firmly advocating for rigid foundation behavior under displacement-controlled criteria. The newly developed computational model transcends traditional limitations by delivering multidimensional output—capturing not merely singular values but the intricate spatial distribution of stress and displacement across the foundation zone. Remarkably, the Optimization Specification C Method achieves a 34% reduction in relative error compared to conventional standards, underscoring its superior accuracy, reliability, and real-world applicability. Critically, under conditions of global horizontal sliding of the arch structure, localized shear failure may initiate within the frontal rock mass adjacent to the stepped foundation. Furthermore, four distinct failure modes have been identified, each intrinsically linked to specific geometric configurations of the stepped block foundation—implying that optimal design must be guided by precise evaluation of the failure angle. By integrating bearing capacity assessments with stringent displacement control benchmarks, a holistic evaluation of foundation performance is achieved. While the current arch bridge foundation design successfully satisfies all load-bearing requirements, its deformation response reveals considerable untapped potential for refinement. Engineering case analyses further confirm that conventional single-dimensional performance checks, though inherently conservative and generally safe, fall short of capturing the full complexity of foundation behavior.

How to cite: Yang, X., Deng, W., and Yang, H.: A Masterful Symphony of Strength and Stability: An Exquisite Analysis System for the Load-Bearing Behavior of Stepped Block Arch Bridge Foundations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18283, https://doi.org/10.5194/egusphere-egu26-18283, 2026.

A swarm of m-scale dikes, made of diabase and porphyritic microgranite, related to a ca. 420 Ma bimodal tholeiitic magmatism crops out in the Rocroi Inlier, a Lower Paleozoic inlier exposed in the Ardenne Allochton (western Rhenohercynian Zone, European Variscan Belt). These dikes are affected by a more or less penetrative cleavage and their magmatic mineralogy has been replaced to various degrees by secondary minerals such as albite, chlorite, sericite, epidote and calcite, as a consequence of Pennsylvanian Variscan deformation and associated low-grade metamorphism. The thickest dikes (thickness from 3-4 to 10-15 m) display a deformation gradient from the border zones which has a penetrative cleavage to the core which is little or even apparently not deformed.

We have conducted measurements of the anisotropy of magnetic susceptibility on samples collected along transversal sections across five thick dikes from the Rocroi Inlier, two made of diabase and three of microgranite. The bulk magnetic susceptibility (Km) has typical paramagnetic values, 5.8-14.0 x 10-4 SI in the diabase and 0.4-6.4 x 10-4 SI in the microgranite, except in the core of one diabase dike where magnetite occurs, ca. 580-890 x 10-4 SI. The corrected anisotropy degree (P’) tends to have high values, up to ca. 1.8, in the deformed border zones and decreases towards the core. This parameter is therefore a proxy of the petrofabric strength. The shape parameter (T) reveals a predominantly oblate magnetic fabric, which suggests a prevailing coaxial deformation, in agreement with a previous finite strain study.

Magnetic foliation in the deformed border zones is parallel to dike margin, as well as to cleavage both in diabase or microgranite and in metapelites at the contact with the intrusion. It rotates a few degrees when moving away from the dike walls. Magnetic lineation is orientated down-dip on the foliation plane and is therefore also slightly deflected across the dikes. The mean magnetic foliation dip, hence the mean lineation plunge is ca. 30-60° to the S-SE. This orientation is roughly similar to that of the main (Variscan) cleavage in the metapelitic host rocks which bears a down-dip stretching lineation. However, magnetic fabric in the dikes and petrofabric in the country rocks outside the contact zone with the intrusions are slightly oblique (up to ca. 30°). Such a discrepancy possibly results from fabric refraction due to competence contrast with the host rocks. Incomplete transposition of the magmatic fabric by the Variscan deformation, as observed in particular in some microgranite samples, could also play a role here, by influencing the orientation of the magnetic fabric.

How to cite: Bolle, O., Bopda Tala, N., and Custine, E.: Heterogeneous Variscan deformation in late Silurian–early Devonian diabase and microgranite dikes of the Caledonian Rocroi Inlier (Ardenne Allochthon, France) quantified using anisotropy of magnetic susceptibility (AMS), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18866, https://doi.org/10.5194/egusphere-egu26-18866, 2026.

EGU26-20706 | ECS | Posters on site | EMRP1.1

From Rock Cuttings to Physical Properties: Integrating Digital Rock Physics and Borehole Data from Traunreut, Southern Germany. 

Angelly Serje Gutierrez, Mirko Siegert, Marcel Gurris, and Erik H Saenger

Digital Rock Physics (DRP) methods are increasingly used to link high‑resolution 3D imaging with the numerical determination of rock properties. In this work, we present new results from the SimBoL project, which applies this approach to drill cuttings from a borehole in Traunreut, southern Germany. The goal is to evaluate the potential of non‑core material for reliable petrophysical characterization relevant to geothermal applications.​

High‑resolution X‑ray computed tomography (CT) scans were segmented to obtain representative digital samples of carbonate cuttings, from which mineral composition, thermal conductivity and permeability were derived. A subset of these properties was computed using an updated numerical solver that incorporates periodic boundary conditions, enabling the treatment of irregular cutting geometries without relying on subvolumes or sample reshaping, and thereby allowing the use of larger rock volumes and a more realistic representation of heat and fluid transport processes than previous approaches restricted to cubic domains.​

The ongoing simulations yield quantitative estimates of rock properties that are compared with available borehole data and complemented by observations from thin sections. The analysis illustrates how digital twins of rock cuttings can deliver additional information on the internal architecture of reservoir rocks, reducing dependence on costly core material and strengthening the conceptual basis for geothermal reservoir characterization.

How to cite: Serje Gutierrez, A., Siegert, M., Gurris, M., and Saenger, E. H.: From Rock Cuttings to Physical Properties: Integrating Digital Rock Physics and Borehole Data from Traunreut, Southern Germany., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20706, https://doi.org/10.5194/egusphere-egu26-20706, 2026.

EGU26-21976 | ECS | Orals | EMRP1.1

Advanced Petrophysical Characterization of Thin-Bedded Reservoirs Through Integrated Laboratory, Well Logging, and Seismic Data 

Sebastian Waszkiewicz, Paulina Krakowska-Madejska, Anna Kwietnak, and Krzysztof Starzec

Thin-bedded Miocene formations of the Carpathian Foredeep represent a major challenge for reliable petrophysical characterization due to strong lithological heterogeneity, high clay minerals content, and the vertical resolution of standard well log interpretations. Accurate assessment of porosity and permeability in such reservoirs is essential for hydrocarbon exploitation, geothermal applications, and the evaluation of Carbon Capture and Storage (CCS) potential.

This study presents an integrated pore-structure modeling workflow applied within a multi-well correlation framework, allowing the transfer and validation of petrophysical models across laterally variable, thin-layered deposits. The methodology combines multiscale laboratory measurements (NMR, nitrogen adsorption, MICP, X-ray CT, and FIB-SEM) with machine-learning–assisted interpretation of well log data to generate high-resolution continuous profiles of porosity and permeability. Models calibrated on core-scale laboratory data are propagated between correlated wells, enabling consistent characterization of reservoir properties beyond a single well.

To increase the geological credibility of the multi-well interpretation, seismic data are incorporated as an independent constraint. Seismic attributes support stratigraphic correlation, identification of thin-bed architecture, and the lateral continuity of petrophysical units. This integration facilitates the upscaling of pore-scale information from laboratory and well log data into a seismic framework, reducing uncertainty related to heterogeneity and thin layering.

The results indicate that the combined use of artificial neural networks, advanced statistical methods, and seismic support significantly improves both vertical and lateral resolution of petrophysical properties in thin-bedded reservoirs. The proposed workflow enables reliable application of pore-network–based models within a multi-well context and provides a scalable approach for reservoir characterization in complex clastic systems. The methodology is particularly relevant for unconventional reservoirs and mature fields considered for CCS or geothermal repurposing, where accurate representation of thin-layered architectures is critical for realistic resource assessment.

How to cite: Waszkiewicz, S., Krakowska-Madejska, P., Kwietnak, A., and Starzec, K.: Advanced Petrophysical Characterization of Thin-Bedded Reservoirs Through Integrated Laboratory, Well Logging, and Seismic Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21976, https://doi.org/10.5194/egusphere-egu26-21976, 2026.

EGU26-317 | ECS | Orals | EMRP1.2

Hygroscopic weakening accelerates the transition to catastrophic failure during brittle creep in clastic rocks 

Rui Wu, Hongpu Kang, Fuqiang Gao, Xiangyuan Peng, Shuangyong Dong, Chenxi Zhao, Bing Li, Kerry Leith, Qinghua Lei, and Paul Selvadurai

Understanding how water influences slow fracture growth in rocks remains a major gap in our ability to predict time-dependent failure. In particular, it is still unclear how moisture-related weakening push a subcritically stressed rock from stable deformation into sudden collapse.

In this study, we investigate how hygroscopic weakening—caused by liquid water entering a notch—affects the creep behavior of a clastic rock loaded below its short-term strength. Using a sandstone beam (400 mm×90 mm×90 mm) in an inverted three-point bending setup, we first load the sample to about 67% of its failure strength more than 5 days, then introduce a controlled water drip directly into the notch.

We track the fracture response using digital image correlation, ultrasonic transmission, acoustic emission, and crack-opening measurements. The results show two distinct stages after water arrives:

  • a rapid increase in crack opening and loss of stiffness, consistent with moisture-driven softening; and
  • a slower but sustained rise in microcracking activity, leading to accelerated creep and, in some cases, catastrophic failure.

In contrast, identical dry beams remain stable over several days, confirming that water—not load alone—initiates the transition to instability.

These findings demonstrate that even small amounts of liquid water can sharply alter the long-term mechanical stability of brittle stressed rocks. This work highlights a potential pathway through which more frequent or intense wetting events could increase the likelihood of sudden rock failure in natural and engineered settings.

How to cite: Wu, R., Kang, H., Gao, F., Peng, X., Dong, S., Zhao, C., Li, B., Leith, K., Lei, Q., and Selvadurai, P.: Hygroscopic weakening accelerates the transition to catastrophic failure during brittle creep in clastic rocks, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-317, https://doi.org/10.5194/egusphere-egu26-317, 2026.

EGU26-338 | ECS | Posters on site | EMRP1.2

Multi-scale control of initial porosity distribution on deformation processes in a heterogeneous porous carbonate rock 

Catherine Dore-Ossipyan, Adriana Quacquarelli, Jean Sulem, Michel Bornert, Alexandre Dimanov, and Andrew King

Understanding the mechanical behavior of porous carbonate rocks is critical for improving reservoir management and developing sustainable energy solutions. Carbonate rocks are formed through complex sedimentary processes and diagenesis, leading to significant microstructural variability at multiple scales, which influences their mechanical properties. This complexity necessitates advanced experimental tools to accurately describe their behavior under various stress conditions. 

Recent studies have demonstrated that strain is accommodated heterogeneously in porous sedimentary rocks, such as sandstones and limestones. Precisely, formation of deformation bands has been observed under various loading conditions in porous limestones which can significantly affect the capacity, i.e., porosity, and thus permeability, of carbonate reservoirs. The inherent multi-scale nature of carbonate microstructure and deformation bands – from the grain to the reservoir scale – leads to a lack of comprehensive and high-quality data on the relationship between deformation modes and microstructure, despite significant advancements in the field. We propose to carry out extensive experimental investigations on a material at multiple scales and various loading conditions. 

This work explores empirically the relationship between the initial porosity distribution of the heterogeneous Saint-Maximin limestone and the deformation modes observed from the micrometer to the centimeter scale. At the standard laboratory centimeter scale, it was shown that the band pattern was controlled by the porosity heterogeneity at the centimeter scale, and initiated preferably in the zones of lower porosity, showing first order control of porosity at this scale. The abundance of SML experimental data and its heterogeneity were key advantages for exploring strain accommodation at lower scales. By conducting a series of in situ tests on smaller, 8 mm in diameter samples, we aimed to elucidate the role of porosity heterogeneity in the onset and propagation of deformation bands, thus enhancing our understanding of the mechanical processes governing carbonate rocks. Ultimately, the results could contribute to improved modeling of multiscale geosystems. 

How to cite: Dore-Ossipyan, C., Quacquarelli, A., Sulem, J., Bornert, M., Dimanov, A., and King, A.: Multi-scale control of initial porosity distribution on deformation processes in a heterogeneous porous carbonate rock, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-338, https://doi.org/10.5194/egusphere-egu26-338, 2026.

EGU26-1649 | ECS | Posters on site | EMRP1.2

Why firn (old snow) quakes - a continuum mechanics theory with granular legacy 

Anne Voigtländer and Bruce Gee

Granular materials compact, increase in density, and degas as they accumulate. This changes the material properties, storage capacities, and fracture mechanics.  We developed a mechanical model for compacting granular old snow.  Based on minimal assumptions and data, we address a general phenomenon in compacting granular medium: propagating ruptures or “firnquakes”.  

Compacting snow becomes firn then ice. As the snowpack consolidates, it transitions from a non-homogeneous granular material to a more elastic continuum material. We propose that the granular legacy produces spatial variations in density, stiffness, and pre-stress. This creates an internal structure of supports in unconsolidated snow at depth. Firn can quake when these supports collapse. By combining granular with brittle fracture mechanics and making use of statistical percolation theory, we can explain the conditioning, triggering, and progression of firnquakes in a bulk homogeneous material, with near constant boundary conditions.

Our model provides means to assess ruptures in granular materials, which unlike firnquakes, can have hazardous consequences, like landslides, avalanches, powder tailing failure. It also provides mechanistic explanations and statistical approaches to assess storage structure and capacity, which, in the case of Antarctic’s firn, has been linked to icesheet disintegration.

How to cite: Voigtländer, A. and Gee, B.: Why firn (old snow) quakes - a continuum mechanics theory with granular legacy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1649, https://doi.org/10.5194/egusphere-egu26-1649, 2026.

EGU26-3514 | Orals | EMRP1.2

Grain-scale 4D visualisation of strain partitioning during brittle creep in sandstone 

Michael Chandler, Xun Li, Alexis Cartwright-Taylor, Ian Butler, Damien Freitas, Birhanmeskel Woldemichael, Alexander Liptak, Robert Atwood, Ian Main, Maria-Daphne Mangriotis, Andrew Curtis, Florian Fusseis, and Mark Chapman
The partition of strain between seismic and aseismic processes, notably brittle creep, is highly variable in both tectonic and induced seismicity settings. The two processes have a complicated relationship, with brittle creep generally being associated with more distributed deformation and dynamic rupture with strain localisation. While the overall macroscopic strain behaviour during this process is reasonably well established, the mechanisms by which localised damage regions develop, interact, and ultimately coalesce to form localised fault zones remain under active investigation. The recent development of in-situ X-ray tomography during rock deformation experiments enables direct, time‑resolved, three‑dimensional interrogation of these processes at sub-grain scale.
 
Here, brittle creep was induced in a water-saturated sample of heavily cemented Clashach sandstone under triaxial conditions (σ3 = 20 MPa, Ppore = 5 MPa) using the University of Edinburgh’s “Stór Mjölnir” deformation rig (Cartwright-Taylor et al., 2022). This triaxial rig is equipped with piezoelectric transducers to monitor acoustic emissions and seismic velocity change, and was mounted on synchrotron beamline I12 at Diamond Light Source, UK. In-situ X-ray microtomography was conducted throughout the creep process with a voxel edge length of 7.91 μm, comfortably smaller than the average grain diameter of ≅ 300 μm. These coupled datasets allow for simultaneous monitoring of changes in seismic velocity, acoustic emissions, macroscopic and grain-scale strains as the sample creeps (Cartwright-Taylor et al., 2022, Mangriotis et al., 2025).
 
Main (2000) proposed a damage mechanics model that explains the three stages of decelerating, steady-state and accelerating creep through a combination of two mechanisms: initial deceleration due to local hardening processes, with later acceleration driven by interactions between cracks. These three stages were observed in the macroscopic axial strain data and seismic velocity variation, which fit the model closely. Digital Volume Correlation was used to observe the strains within the sample throughout creep. During primary creep, these strains are predominantly dilation, with a steep positive correlation between volumetric and shear strains. These dilational strains are strongly localised around where the eventual failure-plane nucleates. As the sample transitions into secondary creep at εz ≅ 1.85%,  vp reduces to around 85% of its initial value. More mixed compaction and dilation strains are observed, again localised around the eventual failure plane. A sharp burst of more widely distributed shear strain is observed at εz ≅ 1.9% as the strain transitions into tertiary creep, and vp falls to around 80% of its initial value. These strains correspond approximately to the onset of acoustic emissions. The DVC strains then revert to a largely dilational mode prior to dynamic failure. This localised combination of dilation and shear strain development, and evolution of their relative importance over time, independently validates the combination of localised hardening and crack interaction proposed by Main (2000).
 
Main (2000); https://doi.org/10.1046/j.1365-246x.2000.00136.x
Cartwright-Taylor et al. (2022); https://doi.org/10.1038/s41467-022-33855-z
Mangriotis et al. (2025); https://doi.org/10.1038/s41598-025-03105-5

How to cite: Chandler, M., Li, X., Cartwright-Taylor, A., Butler, I., Freitas, D., Woldemichael, B., Liptak, A., Atwood, R., Main, I., Mangriotis, M.-D., Curtis, A., Fusseis, F., and Chapman, M.: Grain-scale 4D visualisation of strain partitioning during brittle creep in sandstone, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3514, https://doi.org/10.5194/egusphere-egu26-3514, 2026.

As a giant hydropower hub on the Jinsha River in China, the underground powerhouse and diversion tunnel of the Wudongde Hydropower Station (WHS) pass through phyllite strata. During tunnel excavation, the unloading stress path has a significant impact on the changes in the mechanical properties of the surrounding rock, while the deformation and failure of the rock mass accumulate continuously, making it urgent to conduct an in-depth study on the time-dependent characteristics of mechanical parameters. In view of this, phyllite samples from the engineering site were selected to carry out a comparative study on the instantaneous and long-term mechanical properties under loading-unloading conditions. To simulate the instantaneous effect of unloading during tunnel excavation, triaxial loading-unloading tests on phyllite were performed using the MTS815.03 test system, with synchronous acoustic emission (AE) monitoring. The test results revealed the evolution law of rock strength parameters under different unloading paths and the differences in the micromechanical mechanisms of unloading-induced failure. To simulate the evolution of mechanical behavior during the long-term operation of the tunnel, triaxial creep tests under loading-unloading stress paths were conducted using a TLW-2000 rock triaxial creep testing system. A creep constitutive model was established to describe the evolution relationship between the deformation and failure of the surrounding rock and time, and the degradation characteristics of its long-term strength parameters were clarified. The study indicates that for phyllite tunnels under long-term operation, the long-term degradation effect of mechanical parameters should be taken into account, and it is more reasonable to adopt the obtained long-term triaxial rheological strength parameters to assess the long-term operational stability of the tunnel. The research results provide a technical basis for the stability analysis and excavation support design of the tunnel.

How to cite: Zhu, J.: Study on Instantaneous and long-term Mechanical Properties of Phyllite under Loading and Unloading Conditions at Wudongde Hydropower Station, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4582, https://doi.org/10.5194/egusphere-egu26-4582, 2026.

EGU26-5089 | Orals | EMRP1.2

Time-dependent compaction creep in tuffs from Krafla volcano (Iceland) 

Michael Heap, Kamal Bayramov, Patrick Baud, and Anette Mortensen

Volcanic rock can be subjected to high and fluctuating pressures and stresses associated with volcanic activity and geothermal production. When subject to a high constant stress in the brittle regime (shallow depths), strain and porosity increase as a function of time, eventually leading to macroscopic failure—a process called brittle creep. In the ductile regime (deep depths), rare experiments have shown that strain accumulates and porosity decreases at a constant stress. During this process—called compaction creep—the rates of strain accumulation and porosity reduction decrease as a function of time. Here, we performed triaxial constant strain rate experiments and triaxial compaction creep experiments on three samples of tuff sampled from boreholes drilled into Krafla volcano (Iceland). The tuffs differ in terms of their source depth (~395, ~505, and ~690 m), macroscopic texture (grain size and distribution), and mineral content (different quantities of clay minerals/chlorite). The connected porosities of the tuffs, however, are very similar (0.29–0.35). We first performed X-ray computed tomography on each tuff in order to provide a quantitative description of their microstructure (grain size and distribution, and pore size, distribution, shape, and orientation). Triaxial constant strain rate experiments were then performed at different effective pressures to map out the yield cap for each tuff. Finally, triaxial compaction creep experiments were performed at effective pressures corresponding to the same position on the yield cap for each tuff. The constant differential stress used in these experiments was selected as the same proportion between the onset of inelastic compaction and the inflection point in the stress-strain curve from the constant strain rate experiment performed at the same effective pressure. All three tuffs accumulated strain and lost porosity as a function of time under a constant stress, although the rates of strain accumulation and porosity reduction, and therefore the maximum strain and porosity loss achieved at the end of the experiment, were different. For example, the porosity loss at the end of the experiments (after 100 hours) for the three tuffs was 0.014, 0.015, and 0.023. Because the connected porosity of the three tuffs is the same, differences in their compaction creep behaviour can be explained by differences in their microstructure and mineral content. The time-dependent compaction of porous volcanic rocks, demonstrated here for tuffs, has implications for volcano stability and geothermal production.

How to cite: Heap, M., Bayramov, K., Baud, P., and Mortensen, A.: Time-dependent compaction creep in tuffs from Krafla volcano (Iceland), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5089, https://doi.org/10.5194/egusphere-egu26-5089, 2026.

During uniaxial compression testing, the sample fails macroscopically in the form of longitudinal splitting. This indicates that, although only axial load was applied, internal tensile forces caused the sample to fail. In the classic Mohr-Coulomb failure criterion, these tensile forces are not taken into account and the minimum principal stress is considered to be zero. In our modified Mohr-Coulomb failure criterion, we assume that during a uniaxial compression test, tensile stresses are generated in the rock, causing the specimen to fail. Under this assumption, it is possible to extend the stress state during a compression test into the tensile range. The hypothesis is that during a uniaxial compression test, failure is also determined by the tensile strength perpendicular to the load axis. Based on Mohr-Coulomb theory, it is now possible to determine the cohesion and internal friction coefficient from this stress state, knowing only the compressive and tensile strength of the rock.

This method has been tested for various rock types with known values for cohesion, internal friction coefficients, and tensile and compressive strength. Our method provides a good estimate of the intrinsic rock properties.

We present the theoretical basis for our modified Mohr-Coulomb failure criterion and its applicability to various rock types.

How to cite: Blöcher, G. and Cacace, M.: Estimation of cohesion and internal friction coefficient using a modified Mohr-Coulomb failure criterion., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5143, https://doi.org/10.5194/egusphere-egu26-5143, 2026.

EGU26-5261 | ECS | Orals | EMRP1.2

The effect of fluid chemistry on sandstone’s fracture toughness and frictional strength: Implications for brittle and ductile strength 

Corentin Noël, Patrick Baud, Francesco Lazari, Ghassan Shahin, and Marie Violay

In the upper crust, rock pore spaces may be occupied by fluids of diverse chemical compositions. Pore spaces can be naturally filled with water, carbon dioxide, oil or gas, or artificially saturated with reactive fluid for geo-engineering purposes, including geothermal energy, wastewater disposal, carbon dioxide or hydrogen storage. The presence of water and other fluids modifies the mechanical strength of porous rocks in both the brittle (i.e., localised) and ductile (i.e., distributed) regimes. According to micromechanical models, the strength of porous rock in the brittle regime is controlled by both frictional parameters and fracture toughness of the material, while inelastic compaction by cataclastic pore collapse is governed exclusively by fracture toughness. Experimental studies indicate that the presence of fluid affects the fracture toughness and static friction of limestones and sandstones. Accordingly, for a given rock type, fluid-induced weakening of the rock strength should be explained entirely by a decrease in fracture toughness and/or frictional parameters.

This interpretation is supported by measurements of the mode-I fracture toughness (KIc) and static friction (µs) of sandstones and limestones, under both dry and water-saturated conditions, which allow for the estimation of the uniaxial compressive strength and quantification of the degree of water-weakening. In this context, we investigate the influence of fluids and fluid composition on the mode-I fracture toughness and frictional strength of Adamswiller sandstone. This sandstone was selected because its mechanical behaviour is well-documented in the literature, and because both fluid presence and fluid composition have been shown to affect its response under uniaxial and triaxial compression. We tested a range of fluid-saturated conditions, including dry, deionised water, 6 mol NaCl solution, 0.1 mol HCl solution and 0.1 mol NaOH solution. For KIc, most of the weakening occurs between dry and fluid-saturated conditions, with additional reductions observed for acidic and basic solutions, with the greatest under basic conditions. For a saline solution, the extent of weakening relative to water-saturated conditions is unclear. In contrast, the measured static and peak friction coefficients are unaffected by either the fluid presence or the fluid composition. Incorporating the measured toughness and frictional strength into micromechanical models (wing crack model and pore collapse model) successfully reproduces fluid-weakening under uniaxial and triaxial conditions. The models capture the effective pressure dependence of fluid-weakening in both the brittle and ductile regimes, reproducing the observed strength variation associated with different fluid compositions. This experimental dataset provides new insight that constrains the micromechanical mechanisms governing porous rock deformation in natural and anthropogenic fluid-saturated environments, with direct implications for the safe exploitation of geo-reservoirs.

How to cite: Noël, C., Baud, P., Lazari, F., Shahin, G., and Violay, M.: The effect of fluid chemistry on sandstone’s fracture toughness and frictional strength: Implications for brittle and ductile strength, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5261, https://doi.org/10.5194/egusphere-egu26-5261, 2026.

EGU26-5766 | Posters on site | EMRP1.2

Changes in rock dynamic elastic moduli after thermal cycling in a controlled environment 

Jan Blahůt, Tomáš Lokajíček, Artem Polezhaev, Ondřej Racek, and Marco Loche

Temperature fluctuations can influence the internal stress field of a rock mass, especially in its surficial layer. Inherent properties (mineral composition, porosity, and fracturing) and external forcing (air temperature, humidity, and solar radiation) control the heat flux and temperature within the rock. Long-term thermal forcing, particularly when combined with wetting-drying cycles, can exacerbate rock deterioration and weathering, leading to progressive changes in mechanical properties, as shown by laboratory experiments.

In this study, granodiorite samples from the Požáry field laboratory (Central Czechia) were subjected to thermal cycling in a controlled environment of a climate chamber, with repeated and increasing cycles reaching 80°C, a temperature that was most probably never reached after the rock´s formation.  During the cycling, repeated UPV measurements were made (P and S waves) to observe the changes in their velocity and the inferred dynamic elastic moduli.

The results showed slow but progressive decrease in the P and S wave velocities, suggesting rock damage after only a few cycles. This indicates possible increased rock wear in case of an expected future temperature rise.

How to cite: Blahůt, J., Lokajíček, T., Polezhaev, A., Racek, O., and Loche, M.: Changes in rock dynamic elastic moduli after thermal cycling in a controlled environment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5766, https://doi.org/10.5194/egusphere-egu26-5766, 2026.

 Large-magnitude earthquakes in the continental crust predominantly occur near the brittle–ductile transition zone, where the deformation behavior of rocks plays an important role in earthquake nucleation and energy release.Rocks deforming under high-temperature and high-pressure conditions within the brittle–ductile transition zone may exhibit mechanical responses controlled not only by temperature and stress level, but also by pre-existing microstructural features; in particular, perthitic feldspar, a widespread feldspar solid solution in the crust, commonly contains exsolution-related lamellar structures that may introduce orientation-dependent deformation behavior.Despite its common occurrence in mid-crustal rocks, the influence of pre-existing lamellar fabric orientation on the deformation behavior of perthitic feldspar, especially under brittle–ductile transition conditions, remains poorly constrained by experiments.Based on this background, we conducted high-temperature and high-pressure deformation experiments using a Griggs-type solid-medium apparatus to systematically investigate the deformation behavior of perthitic feldspar with different pre-existing lamellar fabric orientations.Samples were prepared with lamellar orientations at angles of 0°, 45°, and 90° relative to the maximum principal stress, and deformed at a confining pressure of 1 GPa, over a temperature range of 600–1050 °C, at strain rates ranging from 5 × 10⁻⁵ to 2 × 10⁻⁶ s⁻¹. Microstructures of the samples before and after deformation were characterized using scanning electron microscopy and electron backscatter diffraction, and the mechanical responses and microstructural features were compared among samples with different fabric orientations.The mechanical results show significant differences in peak strength among the three lamellar fabric orientations, with sample strength decreasing in the order of 45°, 0°, and 90° at the same temperature.All samples entered a plastic deformation regime above 800 °C (σd<Pc).Microstructural observations reveal that at low temperatures (<900 °C), pervasive brittle cracks crosscut both feldspar phases and are accompanied by localized ductile shear zones; at intermediate temperatures (900–950 °C), cracks are mainly confined within albite grains and are commonly oriented perpendicular to grain boundaries; at high temperatures (>950 °C), samples exhibit bulk plastic flow with a marked reduction in cracking.Notably, samples with a 45° lamellar orientation experienced pronounced bulk fragmentation at 1000 °C and 1050 °C.EBSD results show that K-feldspar does not develop significant changes in crystallographic preferred orientation during deformation, whereas albite exhibits progressively heterogeneous orientation patterns with increasing temperature, consistent with plastic deformation associated with subgrain rotation recrystallization.Together, the mechanical and microstructural results demonstrate that pre-existing lamellar fabric orientation exerts a significant influence on the deformation behavior of perthitic feldspar under brittle–ductile transition conditions, providing experimental constraints on strength anisotropy in feldspar-rich rocks.

How to cite: yaqi, C., jiaxiang, D., and yongsheng, Z.: Deformation behavior of perthitic feldspar under brittle–ductile transition conditions: effects of pre-existing lamellar fabric, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6075, https://doi.org/10.5194/egusphere-egu26-6075, 2026.

EGU26-7457 | Posters on site | EMRP1.2

Unravelling Precursory Rockfall seismic signatures via multiscale clustering analysis 

Sergio Vinciguerra, Guido Maria Adinolfi, Wen Zhou, and Cesare Comina

Seismic monitoring is an effective tool for studying rock mass stability, playing a crucial role in detecting the precursory assessment of damage and cracking processes preceding and accompanying macroscopic failures.

We first present the seismic monitoring results from the Lorgino Quarry in Crevoladossola (NW Italy) where a 6000 m³ rock-fall occurred on January 26, 2023 shortly after deploying a small-aperture array (about 100 meters) of three seismic stations, equipped with a tri-axial, velocimetric sensor and data-loggers sampling at 250 Hz. The rock fall took place about a month after the site-specific seismic array installation at the lithological contact between folded gneisses and a dolomitic limestones unit, mainly composed of dolomites and dolomitic saccharoid marbles. The rockfall seismic signature lasted 15s and the spectral analysis shows the occurrence of multiple sub-episodes of slip triggered by the initial rupture. 

As no obvious correlations between precursory activity and the rockfall occurrence were observed via traditional seismological approaches, we applied an unsupervised deep-learning method that combines a deep scattering network, for automatic feature extraction, with Gaussian mixture model clustering. This approach successfully identified low-amplitude signals occurring nearly one hour before the rockfall, nearly undetectable in raw seismic records and likely associated with a nucleation phase occurring well before the acceleration to failure.

In order to investigate the physical mechanisms driving the nucleation phase, we carried out rock deformation laboratory experiments, where marble cylindrical samples (100x40mm) from the quarry were triaxially loaded in compression to failure at constant effective pressure (20MPa) while an array of 16 Piezoelectric Transducers recorded the ongoing Acoustic Emissions (AE). The time and spatial distribution of AE reveal the nucleation and growth of patches led by limited occurrence of low energy AE events and the coalescence of microfractures into cm-scale macroscopic ruptures planes leading to AE clustering and stress drop and a peak in number of events and energy. Preliminary source mechanism analysis, carried out by developing an automated focal mechanism inversion workflow for AE based on P-wave first-motion, integrating polarity and amplitude measurements, suggests that the inverted focal mechanisms are stable and broadly consistent with the imposed stress conditions, highlighting the potential of the workflow to improve source mechanism quality by identifying and excluding unreliable solutions.

How to cite: Vinciguerra, S., Adinolfi, G. M., Zhou, W., and Comina, C.: Unravelling Precursory Rockfall seismic signatures via multiscale clustering analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7457, https://doi.org/10.5194/egusphere-egu26-7457, 2026.

With the extension of mining and tunneling engineering into deep complex water-bearing strata, the interaction between groundwater and rock mass has become a critical factor governing mechanical excavation efficiency. The presence of water fundamentally alters the rock fragmentation characteristics, and understanding this hydro-mechanical coupling is prerequisite for optimizing conical pick performance. In this study, a comprehensive experimental framework combining macroscopic indentation tests and microscopic characterization was established to evaluate the breakability of twenty distinct lithologies under dry and saturated conditions. The variation of Peak Indentation Force (PIF) and cutting work was monitored, alongside micro-analysis using SEM and XRD to reveal the intrinsic controls of mineral composition and pore structure. The results demonstrate a lithology-dependent bifurcation: porous sedimentary rocks exhibit significant degradation in strength due to pore pressure wedging and chemical softening, whereas dense magmatic rocks remain largely insensitive to saturation. Furthermore, to bridge the gap between experimental data and field application, an Extreme Gradient Boosting (XGBoost) model was used. Feature importance analysis reveals that under water-saturated conditions, the Brittleness Index surpasses hardness as the dominant predictor for rock breakability. This study quantifies the water-weakening mechanism and provides a data-driven approach for predicting cutter performance and improving excavation efficiency in water-bearing environments.

How to cite: Shi, X. and Wang, S.: Experimental investigation and machine learning prediction of water-weakening effects on rock breakability by conical pick, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8640, https://doi.org/10.5194/egusphere-egu26-8640, 2026.

Frost heave and thaw settlement are among the most widespread and destructive geotechnical hazards in cold regions, posing serious threats to the safety and long-term performance of infrastructure. The initiation and evolution of these hazards are highly dependent on the mechanical properties of frozen soils, such as compressive strength, cohesion, internal friction angle, and deformation modulus. These properties are jointly controlled by temperature, ice content, water content, and freeze–thaw cycling, resulting in strong nonlinearity, temporal variability, and spatial heterogeneity. As a result, conventional laboratory testing and empirical approaches often suffer from high cost, low efficiency, and limited applicability in parameter determination and prediction. In recent years, machine learning techniques have been increasingly applied to predict soil mechanical parameters due to their ability to handle multi-source data and capture complex nonlinear relationships. However, the strong temperature sensitivity of frozen soil behavior makes it difficult to achieve high prediction accuracy by solely establishing mappings between temperature–moisture–structural characteristics and mechanical responses. This challenge highlights the necessity of data-driven modeling frameworks that explicitly consider stress states and thermomechanical coupling effects. In this study, a machine learning–based framework was developed to predict the strength characteristics of frozen clay. A total of 116 sets of directional shear test data were used to train and validate four machine learning algorithms. The intermediate principal stress coefficient, principal stress axis orientation angle, mean principal stress, and temperature were selected as input variables, while frozen clay strength was taken as the output. Model performance was systematically evaluated using cross-validation and further verified through comparison with supplementary experimental data. Based on the optimal model, the distribution of frozen clay strength within a multi-dimensional input parameter space was analyzed. In addition, model interpretability techniques were employed to conduct sensitivity analysis, enabling quantitative evaluation of the relative importance of different input parameters. The results demonstrate that machine learning approaches can accurately reproduce the stress–strain behavior and failure strength of frozen clay, while effectively capturing the complex nonlinear relationships between strength and controlling factors. Overall, this study shows that machine learning provides a robust and efficient alternative for predicting frozen soil mechanical parameters. The proposed framework enhances prediction.

How to cite: Wang, D.: Prediction of Frozen Clay Strength Under Different Temperature Conditions Using Machine Learning Approaches, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11103, https://doi.org/10.5194/egusphere-egu26-11103, 2026.

EGU26-11234 | Posters on site | EMRP1.2

Optimization of Tunnel Support Systems in High-Stress Geological Zones: A Case Study of Diamer-Basha Dam 

Umair Aman, Zulfiqar Ali, Sardar Nasir Hussain, Shahid Nazeer, and Muhammad Ayub

Excavating large-scale tunnels in tectonically active regions, such as the Himalayan seismic zone, challenges the stability of underground structures due to high in-situ and induced stresses. The Diamer-Basha Dam (DBD) project involves complex tunneling through heterogeneous bands of granite and diorites, necessitating an engineered support system to mitigate progressive rock mass failure. In Pakistan, the tunnel support often relies on empirical classifications like the Rock Mass Rating (RMR) and Q-system. These systems provide a useful initial estimate; however, their direct application without site-specific calibration frequently results in conservative or over-designed support systems. This study investigates an optimized support framework by integrating empirical characterization with numerical Finite Element Method (FEM) analysis. Using geological data acquired from the site, including face maps and borehole logs, we classified rock mass and simulated its response to excavation using RS2 software. The research specifically evaluates the mechanical efficacy of Fiber Reinforced Shotcrete against optimized combinations of plain shotcrete and active rock bolts. Numerical simulations indicate that the in-situ rock mass possesses sufficient self-supporting capacity in specific zones to allow for a reduction in shotcrete thickness when supplemented with bolting. The models demonstrate that optimized designs maintain the required structural stability while reducing material consumption. These findings suggest that a hybrid empirical-numerical framework offers a cost-effective engineering solution for large excavations. By validating support performance through numerical modelling, this study provides a repeatable framework for optimizing tunnel support in complex geological environments.

How to cite: Aman, U., Ali, Z., Hussain, S. N., Nazeer, S., and Ayub, M.: Optimization of Tunnel Support Systems in High-Stress Geological Zones: A Case Study of Diamer-Basha Dam, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11234, https://doi.org/10.5194/egusphere-egu26-11234, 2026.

EGU26-11286 | ECS | Posters on site | EMRP1.2

Investigating the thermal behavior of exfoliation sheets in granitic cliffs (Yosemite, USA) through laboratory experiments and numerical modeling  

Filippo Giorgi Spreafico del Corno, Federico Agliardi, Riccardo Castellanza, Greg M. Stock, Rebecca Bruschetta, and Brian D. Collins

Yosemite National Park (California, USA) is characterized by high granitic rock walls affected by diffuse rock slope instabilities. These pose high rockfall hazards to roads and threaten the lives of millions of people that every year access the park to visit the natural beauties of Yosemite Valley, walk trails and climb iconic rock walls like El Capitan. Here, rockfalls are chiefly triggered by the progressive failure of portions of exfoliation sheets (“flakes”) bound to the cliff by rock bridges. In this context, identifying potentially unstable flakes is crucial for risk mitigation, yet the field characterization of such flakes remains difficult, highlighting the need for remote sensing mapping methods.

At the southeastern face of El Capitan, in situ time-lapse infrared thermographic (IRT) surveys, conducted in October 2024, revealed that exfoliation sheets cool faster than the surrounding rock mass heated by the same daily solar forcing. To lay foundations for a remote detection methodology, we carried out a combined laboratory and numerical study of the IRT signature of daily heating and cooling of exfoliation sheets and the underlying physical processes.

We conducted 37 laboratory experiments in a controlled setup, where the cooling of 20 cm by 20 cm granite slabs with variable thickness (1-6 cm) and opening of a simulated exfoliation joint (2-54 mm), oven-heated at 85°C, is monitored by contact thermocouples and a high resolution thermal camera. For each tested combination of slab thickness and joint aperture, we recorded detailed temperature time series and modelled cooling curves using the lumped capacitance solution of Newton’s law of cooling.

Experimental results show that, until a threshold value of the thickness/aperture ratio is reached, IRT can detect a dependence between the cooling rate of the external slab face and the aperture of the simulated exfoliation joint, with two contrasting trends. For very small aperture, cooling speed decreases with aperture. Beyond a certain aperture value, varying with slab thickness, the slab face cools faster as joint aperture increases.

To investigate the physical processes underlying this behaviour, we reproduced our experiments by 2D and 3D finite-element numerical simulations with the software Temp/W-GeostudioTM, considering different conditions (i.e. initial temperature of the cliff rock behind the flake, conduction, and air convection parameters). Model results suggest that convective heat transport in the open simulated joint strongly controls the thermal energy dissipation within the cooling flake. For very small joint apertures or limited convective circulation, the insulating effect of air results in slower flake cooling. However, for increasing joint aperture and thus greater air convection, the results indicate more effective heat dissipation and associated faster cooling. Our study provides a quantitative framework towards the development of remote mapping of unstable rock features upon proper methodology upscaling to in situ conditions.

 

How to cite: Giorgi Spreafico del Corno, F., Agliardi, F., Castellanza, R., Stock, G. M., Bruschetta, R., and Collins, B. D.: Investigating the thermal behavior of exfoliation sheets in granitic cliffs (Yosemite, USA) through laboratory experiments and numerical modeling , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11286, https://doi.org/10.5194/egusphere-egu26-11286, 2026.

Fault zones in clay-rich formations play a critical role in controlling deformation, fluid flow, and stability in both natural and engineered subsurface systems, including earthquake rupture, underground storage, and radioactive waste disposal. However, the coupled hydro-mechanical behavior of natural fault rocks remains poorly constrained due to the difficulty of obtaining representative samples and performing fully coupled laboratory experiments. Here, we present results from petrophysical and fully hydro-mechanically coupled triaxial compression tests on preserved natural fault material from scaly clay sections of the Main Fault intersecting the Opalinus Clay formation at the Mont Terri Underground Research Laboratory, Switzerland.

The hydraulic properties of scaly clay Opalinus Clay were measured using flow-through experiments on back-saturated specimens. Permeability coefficients determined sub-parallel to the orientation of bedding and tectonic shears are up to three orders of magnitude larger than those of the intact rock. The shear experiments were conducted under undrained conditions at different effective confining stresses, allowing direct observation of stress–strain behavior, pore pressure evolution, and effective stress paths up to large axial strains. In contrast to intact Opalinus Clay, the faulted scaly clay exhibits continuous strain hardening without a distinct peak stress or post-peak weakening. Deformation is distributed and accommodated by the reactivation of multiple pre-existing tectonic micro-shear. The shear strength analysis within a Mohr–Coulomb framework reveals that the scaly clay fabric has effectively zero cohesion and a shear strength that is lower than even the residual strength of intact Opalinus Clay. Microstructural observations confirm that deformation proceeds through distributed sliding along an anastomosing network of polished micro-shears surrounding undeformed microlithons.

These results demonstrate that inherited fault-zone fabric exerts a first-order control on both mechanical strength and hydro-mechanical coupling in clay-rich faults. Incorporating fabric-and stress-dependent behavior as well as critical-state deformation into constitutive models is therefore essential for realistic predictions of fault reactivation, pore pressure evolution, and long-term stability of low-permeability clay formations.

How to cite: Winhausen, L., Ziegler, M., and Amann, F.: The hydro-mechanical coupling, reduction of effective strength, and critical state shearing of faults: Evidence from laboratory testing on natural fault rock, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13046, https://doi.org/10.5194/egusphere-egu26-13046, 2026.

EGU26-13221 | ECS | Orals | EMRP1.2

Resolving Thermo-Hydro-Mechanical Coupling and Progressive Damage in a Metastable Toppling Rock Slope using Integrated Fiber-Optic Monitoring 

Mingyue Yuan, Jacob Hirschberg, Nicolas Oestreicher, Larissa de Palézieux, and Jordan Aaron

The behaviour of slowly moving rock slope instabilities in alpine regions is governed by the interaction between inherited structural discontinuities and externally imposed environmental forcing, yet the mechanisms linking these controls across scales remain poorly constrained due to the lack of continuous subsurface observations. Rock slope toppling represents a typical form of such structure-controlled deformation. Here, we present a comprehensive investigation of a structurally complex toppling rock slope in pre-Variscan metamorphic units in the Bedretto Valley (Swiss Alps). This landslide is intersected by the unlined Bedretto Tunnel over a length of approximately 450 m. The presence of the tunnel and the associated facilities of the Bedretto Underground Laboratory provides a unique opportunity to resolve spatially variable deformation.

To understand the controls on the motion of this landslide, we installed a multi-parameter monitoring network, which integrates surface and subsurface measurements. It combines meteorological stations covering the toppling crown and toe, sectional groundwater pressure monitoring, and a 2-km-long distributed fiber optic sensing (DFOS) cable anchored along the Bedretto Tunnel. This configuration provides a unique internal view of deformation within the rockmass, enabling continuous, decimeter-scale observations of microstrain and temperature beneath up to 1500 m of overburden.

The measurements reveal two distinct deformation responses of the landslide. First, reversible, centimeter-scale strain oscillations correlate with surface temperature fluctuations but exhibit anomalously high amplitudes and penetration depths, which cannot be explained solely by conductive heat transfer. This points to a non-local thermoelastic response, whereby far-field thermal stresses are generated and anisotropically transmitted through the fracture network within the rockmass. Superimposed on this cyclic thermoelastic background, the data reveal discrete, irreversible strain steps near critical fracture zones. These steps temporally coincide with major seasonal hydrologic events including sustained snowmelt and intense rainfall when a two-layer bucket model predicts corresponding peaks in groundwater storage and pressure transients. This correlation provides direct evidence for hydro-mechanically driven, progressive damage within the fracture network of the slope.

Multivariate decomposition of the deformation time series isolates not only the dominant thermo-hydraulically driven cyclic signal, but also residual components characterized by spatially variable, and locally opposing, monotonic strain trends. These opposing trends are partially explained by the mechanical and geometrical heterogeneity of the fracture network and reveal the accumulation of progressive inelastic deformation. Beyond direct thermal or hydraulic forcing, such components suggest a creep-like weakening mechanism of the rockmass under quasi-static gravitational stress.

These findings reveal the dynamics of a coupled thermo-hydro-mechanical system, in which seasonal forcing drives both reversible deformation and irreversible damage. The study thus highlights the critical role of discontinuities in controlling slope behavior, showing how transient hydrology and thermal cycling progressively degrade rockmass strength along pre-existing fractures and joints, ultimately weakening large rock slope failures.

How to cite: Yuan, M., Hirschberg, J., Oestreicher, N., de Palézieux, L., and Aaron, J.: Resolving Thermo-Hydro-Mechanical Coupling and Progressive Damage in a Metastable Toppling Rock Slope using Integrated Fiber-Optic Monitoring, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13221, https://doi.org/10.5194/egusphere-egu26-13221, 2026.

EGU26-15252 | ECS | Posters on site | EMRP1.2

Multiscale controls on cyclic damage and elastic memory in heterogeneous rocks from a porphyry copper system 

Matías Clunes, Francisca Valdés, Tomás Roquer, Jorge Cortez, Martín Garrido, John Browning, Roberto González, and Luis Felipe Orellana

Understanding damage accumulation under cyclic loading is critical for assessing the stability of deep excavations and heterogeneous crustal rocks subjected to repeated stress perturbations. Subvolcanic and volcanic lithologies typical of porphyry copper systems, and analogous to shallow volcanic crust, exhibit strong mineralogical and structural heterogeneity due to intrusive processes, veining, and hydrothermal alteration, challenging models derived from homogeneous rocks. We present results from uniaxial and triaxial cyclic loading experiments on five lithologies from the El Teniente porphyry copper deposit (tonalite, diorite, porphyritic dacite, veined andesite, and hydrothermal breccia), conducted under confining pressures up to 25 MPa and coupled with continuous acoustic emission (AE) monitoring. Cycles of increasing stress amplitude were used to quantify stiffness degradation and acoustic memory through the Felicity Ratio (FR). Elastic moduli were derived from unloading branches, allowing direct comparison with elastic reversibility frameworks proposed for crystalline rocks. Homogeneous to moderately heterogeneous lithologies exhibit gradual stiffness loss and limited departure from elastic reversibility, whereas strongly heterogeneous rocks display pronounced stiffness fluctuations, early deviation from elastic behaviour, and broad FR dispersion, indicating intermittent strain localization and partial loss of elastic memory. Increasing confinement reduces mechanical and acoustic scatter, highlighting the stabilizing role of lateral stress. Ongoing work integrates photogrammetry-based quantification of grain-size distributions, vein density, vein thickness variability, and alteration intensity. These micro- and mesoscale descriptors are used to explore correlations with mechanical degradation rates and acoustic reactivation patterns observed during cyclic loading. This combined mechanical–microstructural approach aims to clarify how lithological heterogeneity governs the style, rate, and intermittency of cyclic damage in subvolcanic crust, with implications for deep mining stability and stress cycling in volcanic systems.

How to cite: Clunes, M., Valdés, F., Roquer, T., Cortez, J., Garrido, M., Browning, J., González, R., and Orellana, L. F.: Multiscale controls on cyclic damage and elastic memory in heterogeneous rocks from a porphyry copper system, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15252, https://doi.org/10.5194/egusphere-egu26-15252, 2026.

EGU26-15305 | Orals | EMRP1.2

Alteration-related damage thresholds in cyclically loaded rocks from deep mining environments 

Francisca Valdés, Matías Clunes, Tomás Roquer, Jorge Cortez, Martín Garrido, John Browning, and Luis Felipe Orellana

Hydrothermal alteration exerts a first-order control on the mechanical behaviour of rocks in deep mining environments by modifying mineralogical composition, grain bonding, and internal structures. In porphyry copper systems, quartz–sericite, potassic and chloritic alteration produces strong contrasts between mechanically competent and weak mineral phases, influencing damage accumulation and failure under cyclic stress conditions. However, experimental constraints on how alteration intensity governs mechanical degradation and acoustic response during cyclic loading remain limited. We investigate the mechanical and acoustic behaviour of rocks exhibiting variable degrees of alteration from a porphyry copper deposit. A total of 57 specimens, classified according to their alteration intensity, were subjected to single-cycle and multi-cycle compression tests under unconfined and confined conditions (σ₃ = 15 MPa). Acoustic emission (AE) monitoring was performed continuously to track microcrack activity and damage evolution during loading. Analysis of the unloading modulus throughout cycles reveals a progressive stiffness degradation that correlates with internal damage accumulation. In general, ‘perfect elasticity’, where loading and unloading gradients converge, is only observed at low stress levels, typically between 20% and 40% of the peak strength. These results contrast with previous studies on more homogeneous rocks, where a broader elastic range were reported. Our findings indicate that beyond 40% threshold, the divergence between loading and unloading moduli increases sharply as a function of cycle accumulation. Samples enriched in softer mineral phases (sericite-rich) exhibit distinct acoustic signatures that reflect a more distributive damage mechanism, whereas quartz- and K-feldspar–dominated rocks, characterized by higher mineral hardness, show a greater damage and microcrack accumulation. This is quantitatively supported by the Felicity Effect analysis: under unconfined conditions, rock dominated by harder mineral phases exhibit lower Felicity Ratio (FR) values, indicating significant pre-peak damage. However, the introduction of a 15 MPa confining pressure leads to a homogenization of the FR across all alteration intensities, as the external stress suppresses micro-cracking regardless of the initial mineralogical heterogeneity. Ongoing analysis explores relationships between alteration degree, mineralogical composition, cyclic damage thresholds, and post-test fracture patterns. By integrating mechanical measurements and acoustic emission data, this work aims to clarify how hydrothermal alteration governs damage accumulation and failure processes in heterogeneous rocks subjected to cyclic stressing, with implications for deep mining stability and induced seismicity.

How to cite: Valdés, F., Clunes, M., Roquer, T., Cortez, J., Garrido, M., Browning, J., and Orellana, L. F.: Alteration-related damage thresholds in cyclically loaded rocks from deep mining environments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15305, https://doi.org/10.5194/egusphere-egu26-15305, 2026.

EGU26-17417 | ECS | Orals | EMRP1.2

Dense ultrasonic imaging of thermo-mechanical stress changes in a limestone cliff 

Alex Rolland, Romain Rousseau, Noélie Bontemps, Juliane Starke, Ludovic Moreau, Laurent Baillet, and Eric Larose

Rock fracturing driven by temperature fluctuations, rainfall, and freeze–thaw cycles governs both long-term landscape evolution and the onset of rock-slope instabilities. However, the thermo-mechanical stress field that develops within the first decimeters of exposed rock—and its role in sub-critical crack growth—remains poorly constrained, largely because it cannot be directly observed at relevant spatial and temporal scales in-situ.

We present a new dense ultrasonic monitoring experiment designed to image near-surface stress, rigidity, and damage in an unstable limestone cliff. The system consists of more than 50 permanently installed ultrasonic transducers deployed over a 4 m² area on a 50-m-high limestone pillar located in the foothills of Larzac, southern France. Half of the sensors operate as emitters and half as receivers, allowing repeated, highly redundant measurements of travel times and waveforms across hundreds of ray paths. Using acousto-elasticity, temporal changes in ultrasonic velocity provide a quantitative proxy for stress and crack evolution, while waveform decorrelation enable tracking of micro-damage and scattering.

The high spatial density of the array enables 2-D and potentially 3-D tomographic imaging of stiffness and damage within the rock surface layer, resolving gradients that are invisible to sparse instrumentation or bulk resonance methods. First results reveal pronounced diurnal velocity variations that correlate with surface temperature and solar radiation, indicating strong thermo-elastic control on near-surface stress and fracture opening.

This new monitoring approach opens the door to direct, time-lapse imaging of climate-driven damage in rock slopes, providing a critical link between environmental forcing, sub-critical cracking, and the progressive weakening that precedes rockfall and cliff collapse.

This work was funded by the European Research Council (ERC) under grant No. 101142154 - Crack The Rock project.

How to cite: Rolland, A., Rousseau, R., Bontemps, N., Starke, J., Moreau, L., Baillet, L., and Larose, E.: Dense ultrasonic imaging of thermo-mechanical stress changes in a limestone cliff, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17417, https://doi.org/10.5194/egusphere-egu26-17417, 2026.

EGU26-17519 | ECS | Orals | EMRP1.2

Impact of creep mechanisms on stress and deformation behaviour around salt caverns 

Gaurav Jain, Brecht Wassing, Suzanne Hangx, Jan Ter Heege, and Hans de Bresser

Salt caverns are formed by solution mining and may be used for energy storage purposes after the production phase. During the operational lifetime, and in particular during abandonment, the spatial and temporal distribution of stress changes and deformation around caverns leads to convergence of salt around the caverns. In turn, this may lead to surface subsidence and potentially affect cavern integrity. Deformation around salt caverns is governed by different creep mechanisms, encompassing transient and steady-state creep stages. Steady-state creep is governed by a combination of dislocation and diffusion creep mechanisms. Deformation due to dislocation creep is dominant at relatively high stresses, whereas grain size-sensitive diffusion creep, particularly pressure solution, contribute significantly at low stresses. When modelling rock salt behaviour, these mechanisms need to be properly accounted for. Recently, studies have suggested that a threshold differential stress may exist below which pressure solution does not take place, which needs to be accounted for. In addition, dynamic recrystallisation may take place through grain boundary migration, driven by differences in energy stored in neighbouring grains due to dislocation creep strain. The process of grain boundary migration reduces the (work hardening) energy in the system as old grains are consumed by new ones, causing weakening. Furthermore, incorporation of transient creep is generally based on the description given in the Munson and Dawson model.

In this study, we aim to simulate different cavern operation phases, such as leaching, production, and abandonment, to analyse the effect of transient creep, pressure solution creep and its threshold stress on the stress and deformation evolution around the cavern. The coupled effects of these complex creep characteristics on cavern behaviour have not yet been studied in detail. Such, more extensive coupling, are needed to better align laboratory- and field-based observations of salt mechanical behaviour, and apply it to large-scale numerical models. The commercial mechanical simulator FLAC (Fast Lagrangian analysis of continua) has been used to develop a 2D model for a single cavern system, which can be used to examine cavern convergence, subsidence and cavern integrity. An empirical model is used to define the threshold strain limit for dynamic recrystallisation by grain boundary migration, analogous to the Munson-Dawson strain limits for transient creep.

The results show a significant effect of pressure solution creep on stress and deformation behaviour around the cavern. In the production phase, the transient creep does not show any significant effect on cavern behaviour; however, it could be important under varying loading conditions. The extent and magnitude of convergence and subsidence are dependent on the rate of pressure solution creep and its threshold stress. A preliminary analysis of the onset of the dynamic recrystallisation around the cavern suggests that DRX may be active in the lower regions of the cavern.

How to cite: Jain, G., Wassing, B., Hangx, S., Ter Heege, J., and de Bresser, H.: Impact of creep mechanisms on stress and deformation behaviour around salt caverns, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17519, https://doi.org/10.5194/egusphere-egu26-17519, 2026.

EGU26-17611 | Posters on site | EMRP1.2

Acoustic Fingerprints - Tracing Irreversible Damage in Natural Cliffs 

Juliane Starke, Romain Rousseau, Alex Rolland, Laurent Baillet, and Eric Larose

Progressive damage and failure in rock masses is governed by multi-scale processes ranging from micro-crack growth to meter-scale fracture opening. We present an active acoustic monitoring approach that captures these evolving processes through time-lapse waveform fingerprinting, providing a quantitative measure of the temporal evolution of rock mass stiffness and scattering properties.

We deployed acoustic sensors on three highly fractured rock cliffs (two limestone sites in southern France and one gneiss site in western Switzerland) and conducted repeated active acoustic measurements every few minutes over periods of several weeks to more than one year. Each source-receiver path yields a unique acoustic response whose complexity increases with fracture density and scattering. By tracking phase shifts and waveform distortions, we 'draw' time-lapse waveform fingerprints that are highly sensitive to small changes in crack density, fracture aperture, and contact stiffness.

The waveform fingerprints reveal strong repeatability under similar meteorological conditions, with coincident patterns observed on days sharing comparable temperature and moisture regimes. Distinct fingerprints emerge under different rock cracking and damage states reflecting reversible thermo-hydro-mechanical effects. Some rocks are indeed more reactive to external forcings than others. At longer timescales, partial but incomplete recovery of the fingerprints is observed. In the one-year data set, major fingerprint features reappear under similar climatic conditions, but with persistent residual changes, indicating the accumulation of irreversible damage within the rock mass.

Future work could apply diffuse acoustic wave spectroscopy and acoustic correlation-based imaging to spatially locate damage and quantify fracture growth, enabling the transition from qualitative fingerprints to quantitative maps of rock degradation.

How to cite: Starke, J., Rousseau, R., Rolland, A., Baillet, L., and Larose, E.: Acoustic Fingerprints - Tracing Irreversible Damage in Natural Cliffs, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17611, https://doi.org/10.5194/egusphere-egu26-17611, 2026.

EGU26-19556 | ECS | Orals | EMRP1.2

The role of veinlets in the unconfined behavior of El Teniente Mine rock samples: Implications for mining-induced rockmass failure. 

Franco Robbiano, Marie Violay, Luis Felipe Orellana, Antoine Guggisberg, and Edouard Heinkel

El Teniente, located in central Chile, is the largest underground copper mine in the world, with ore extraction reaching depths of up to one thousand meters below the surface. The primary ore body is hosted in volcanic rocks of basic composition, extensively intersected by a stockwork of closely spaced veins. At present, the combination of the regional stress regime, localized stress concentrations around excavations, and the heterogeneous nature of the veined rock mass poses significant challenges to operational safety, particularly when considering an extension of the mine’s productive life. Discontinuities, ranging from large-scale faults to small-scale veins, are closely linked to failure processes in mine excavations. In highly homogeneous, intact rock, spalling failure in tunnels is typically initiated at about 50% of the rock’s uniaxial compressive strength (UCS). This relationship is not consistently observed in veined rocks, where standard UCS tests often fail to account for the mechanical influence of discontinuities during deformation. In this study, an experimental setup that integrates four strain gauges, acoustic emission (AE) monitoring, and digital image correlation (DIC) during uniaxial compressive strength (UCS) testing was developed. The method was applied to 20 mm-diameter cylindrical rock specimens from El Teniente to investigate the role of sulfide-rich veins in rock deformation. Samples were selected to minimize the occurrence of multiple veins, containing instead a single primary vein (< 4 mm thick) oriented between 0° and 90° relative to the axial loading direction. Particular emphasis was placed on strain partitioning, with DIC employed to obtain full-field strain measurements, enabling the quantification of strain differences between the rock matrix and the veins. Experimental results indicated that veins accommodated greater strains than the surrounding rock matrix during both the elastic and plastic regimes. All the samples shown a rotation of the local stress tensor on the vein when reaching the onset of dilatancy. Veins oriented between 0 to 40° yielded before the bulk material, with yield onset occurring at 50-60% of the UCS. These findings suggest that precursory shear strain within favorably oriented veins, evidenced by the onset of AE activity, dilatancy and DIC, may play a critical role in initiating rockmass failure at excavation boundaries.

How to cite: Robbiano, F., Violay, M., Orellana, L. F., Guggisberg, A., and Heinkel, E.: The role of veinlets in the unconfined behavior of El Teniente Mine rock samples: Implications for mining-induced rockmass failure., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19556, https://doi.org/10.5194/egusphere-egu26-19556, 2026.

EGU26-2082 | ECS | Orals | EMRP1.3

Illuminating Fluid-Induced Fault Reactivation: Laboratory Insights into Injection-Rate Control on Slip Evolution and Seismic Nucleation 

Federico Pignalberi, Julian Osten, Paul Selvadurai, Elena Spagnuolo, Mohammadreza Jalali, and Florian Amann

Understanding how fluid injection perturbs stressed faults and triggers induced seismicity has become an urgent challenge in geophysics and hazard mitigation. Observations from subsurface fluid injection associated with geoenergy exploitation show that variations in injection pressure and rate and injected volume can strongly modulate seismicity rates and magnitudes. Yet, comparable injection operations may result in stable creep, slow slip, or dynamic rupture, highlighting persistent gaps in our understanding of the physical processes governing fluid-driven fault reactivation.

Here, we investigate fluid-induced fault reactivation through decimetric-scale laboratory experiments on granite samples containing a 45° precut fault. Experiments are conducted in a biaxial apparatus under critically stressed conditions at 3 MPa normal stress, with independent control of normal and shear stresses. Fluids are injected directly into the fault surface while fault slip is measured using fibre-optic sensors (mini-SIMFIP) installed across the fault. Seismic activity is monitored through passive acoustic emission recordings, and repeated active ultrasonic surveys are performed throughout the experiments to track wave velocity changes and map fluid diffusion along the fault.

By systematically varying the injection rate, we observe a clear transition from aseismic creep to slow slip and dynamic rupture. In all cases, fault slip nucleates at the injection point and subsequently propagates within the pressurized region of the fault. High injection rates generate localized overpressure near the injection point, triggering abrupt and seismic fault reactivation. During high-rate injection, we observe a pronounced drop in P-wave velocity, indicating strong mechanical perturbation of the fault zone, followed by a progressive velocity increase as fluids diffuse along the fault. In contrast, low injection rates lead to stable, aseismic slip confined to the pressurized zone, while intermediate rates produce a progressive reactivation sequence in which slip initiates aseismically, evolves into slow slip, and eventually transitions to dynamic rupture as the pressurized region expands.

Our results show that injection rate governs fault slip behavior by controlling where slip nucleates and whether it remains confined to, or propagates beyond, the pressurized zone and accelerates dynamically.

How to cite: Pignalberi, F., Osten, J., Selvadurai, P., Spagnuolo, E., Jalali, M., and Amann, F.: Illuminating Fluid-Induced Fault Reactivation: Laboratory Insights into Injection-Rate Control on Slip Evolution and Seismic Nucleation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2082, https://doi.org/10.5194/egusphere-egu26-2082, 2026.

EGU26-2718 | ECS | Posters on site | EMRP1.3

Development of hydrothermal high-velocity rotary shear apparatus in Kochi, Japan: towards understanding fault slip behavior in the seismogenic zone environment 

Hanaya Okuda, Wataru Tanikawa, Yohei Hamada, Keishi Okazaki, John Bedford, Miku Hidaka, and Takehiro Hirose

In Kochi, JAMSTEC, Japan, we have developed rotary shear apparatuses to understand fault slip behavior of geologic materials at coseismic slip rates. However, coseismic fault behavior under hydrothermal conditions has remained challenging to reproduce in the laboratory. To address this issue, we developed a novel apparatus (HDR: hydrothermal rotary shear apparatus) in 2017, which is capable of high-velocity slip (~2 m/s) at temperatures of up to 600 ℃ and pore fluid pressures of up to 120 MPa. Using this apparatus, we have successfully carried out hydrothermal high-velocity friction experiments on various types of materials, including bare gabbro surfaces and gouges derived from quartz, gabbro, granite, olivine, calcite, and clay minerals under a wide range of pressure-temperature-velocity conditions. The experimental data obtained under hydrothermal conditions are sometimes markedly different from those typically observed in room-temperature experiments due to dynamic changes in fluid properties and chemical reactions in supercritical water. Further understanding of coupled interactions between fault slip, frictional heat, fluid properties, chemical reactions, etc. under hydrothermal conditions will be essential for constraining fault slip behavior in seismogenic-zone settings. In this presentation, we introduce some of our latest results obtained using HDR.

How to cite: Okuda, H., Tanikawa, W., Hamada, Y., Okazaki, K., Bedford, J., Hidaka, M., and Hirose, T.: Development of hydrothermal high-velocity rotary shear apparatus in Kochi, Japan: towards understanding fault slip behavior in the seismogenic zone environment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2718, https://doi.org/10.5194/egusphere-egu26-2718, 2026.

EGU26-3257 | ECS | Posters on site | EMRP1.3

Thermo-hydro-mechanical-chemical modeling of synthetic wet gouges sheared at experimental seismic slip under fluid drainage conditions 

Yu-Qing Huang, Li-Wei Kuo, Chien-Cheng Hung, and Thi Trinh Nguyen

Understanding dynamic weakening is of paramount importance because it involves thermally triggered physical-chemical processes that reduce the fault frictional resistance and facilitate earthquake propagation. Investigating the evolution of temperature (T), pore fluid pressure (Pf), and chemical reactions during slip therefore allows exploration of dynamic weakening mechanisms. However, direct in situ measurements of T and Pf within slip zones remain technologically challenging in laboratory high-velocity rotary shear experiments. Consequently, numerical simulations constrained by mechanical data are essential for inferring these critical parameters. We utilize a series of rotary-shear mechanical data on a combination of kaolinite and quartz. The experiments are conducted under undrained/drained conditions with thermocouples for temperature measurements. On the basis of these data, we develop a Thermo-Hydro-Mechanical-Chemical (THMC) modeling framework using COMSOL Multiphysics to estimate physical conditions within the Principal Slip Zone (PSZ) and to infer dynamic weakening mechanisms responsible for the observed frictional behavior. Under undrained conditions, the friction coefficient (µ) reaches a peak friction (µp) at ~0.28 and undergoes abrupt weakening, followed by a steady-state low-friction (µs) at ~0.1. This behavior corresponds to a measured T stabilizing at 320–360°C and a simulated Pf rapidly increasing and is maintained at ~2.4 MPa. It suggests that frictional heating induces pore water pressurization. Under drained conditions, µ reaches a µp ~0.3 at 0.7s and undergoes abrupt weakening during 1.2-1.7s, maintains µs ~0.17 between 2-4s and followed by a re-strengthening behavior at 4s. µ was accompanied by the changes of T and Pf. T increased to ~280°C at 1.2s, followed by a decrease to ~200°C. Meanwhile, the simulated Pf achieved the highest value (~1.9 MPa) at 1.2s and gradually decreased and reached a relatively lowest value (~0.3 MPa) at 4s due to the pore fluid drainage. Whether Pf is present is corresponding to the weakening and re-strengthening times. In addition, microstructural and mineralogical observations show thermal decomposition of kaolinite. Because thermal decomposition is a strong endothermic reaction, the temperature decreases during the later stages of the process due to the thermal decomposition of kaolinite. We suggest that thermal pressurization operates as the dynamic weakening mechanism during the initial slip stage, consistent with theoretical predictions and experimental documentation of thermal pressurization during rapid shear, as described by Rice (2006) and Ferri et al. (2010). Later, thermal pressurization ceases under drained conditions, resulting in complex frictional behavior. In general, our study provides essential insights into the dynamic weakening mechanism during experimental seismic slip. In addition, we suggest that drainage conditions may influence frictional behavior by affecting the generation and maintenance of pore fluid pressure during seismic slip.

How to cite: Huang, Y.-Q., Kuo, L.-W., Hung, C.-C., and Nguyen, T. T.: Thermo-hydro-mechanical-chemical modeling of synthetic wet gouges sheared at experimental seismic slip under fluid drainage conditions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3257, https://doi.org/10.5194/egusphere-egu26-3257, 2026.

EGU26-4224 | ECS | Posters on site | EMRP1.3

Mechanisms of failure in a fluid-saturated fault gouge subject to cyclic pore-pressure oscillations 

Pritom Sarma, Stanislav Parez, Renaud Toussaint, and Einat Aharonov

While dynamic fluctuations in effective normal stress affecting fault zones are ubiquitous, arising from both complex natural phenomena like remote dynamic triggering of earthquakes and anthropogenic activities like industrial subsurface fluid injection, the precise influence of these perturbations and specifically their frequencies, on the macroscopic fault strength remains insufficiently characterized.The frequency of these pore-pressure variations is likely a key factor setting the timescale for the drained-to-undrained transition, thereby driving markedly different mechanical responses.

In this work, we present results from a coupled hydromechanical-discrete element model simulating a pre-stressed, fully saturated granular fault gouge subject to cyclic pore-pressure variations across three orders of magnitude in frequency. We observe that fault failure consistently occurs before the system reaches the traditional Mohr-Coulomb failure criterion. This early failure indicates that additional dynamic mechanisms, often neglected in effective stress analyses, play a dominant role in triggering instability. We investigate the driving forces responsible for this pre-Mohr-Coulomb failure and find they evolve distinctly with frequency. We evaluate three primary candidates driving this behavior: 1) seepage forces arising from the pore-pressure gradients, 2) contact weakening induced by granular agitation (vibration), and 3) inertial effects driven by acceleration from cyclic pore-pressurization. Our analysis isolates the contribution of each mechanism across the frequency spectrum, offering a new physical basis for understanding why dynamic pore-pressure perturbations can trigger slip earlier than what static friction laws predict.

How to cite: Sarma, P., Parez, S., Toussaint, R., and Aharonov, E.: Mechanisms of failure in a fluid-saturated fault gouge subject to cyclic pore-pressure oscillations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4224, https://doi.org/10.5194/egusphere-egu26-4224, 2026.

EGU26-6001 | ECS | Orals | EMRP1.3

A Multi-Scale Approach to Fault-Valve Systems and Their Evolution 

Oussama Larkem, Luc Scholtès, and Fabrice Golfier

Cyclic fluid injection can promote repeated fault reactivation and transient permeability changes, a behavior often discussed within the fault-valve concept where faults alternate between acting as hydraulic barriers and conduits. Such cycles are relevant to both natural hydrothermal systems and industrial activities that modify pore pressure in the subsurface.

The complex evolution of fault permeability and strength during and after fault reactivation calls for a more complete description of the underlying physical processes. Current state-of-the-art fault reactivation models generally represent these weakening and strengthening mechanisms at the macroscopic scale using phenomenological laws, such as the widely used rate-and-state framework. Although these formulations have proven successful in reproducing some observed fault behaviors, they rely on empirically determined parameters and still leave part of the relevant physics insufficiently described.

Here we investigate these processes using a discrete element method (DEM) approach coupled with a pore-scale finite volume (PFV) scheme. Similarly to the framework proposed by Nguyen et al. (2021), the DEM models the granular gouge, while PFV simulates pore-pressure evolution and fluid flow through the evolving pore geometry, with full two-way coupling between solid deformation and fluid pressure, thus relating the macroscopic response of the system to the micromechanical phenomena at work.

Using this coupled approach, we simulate both monotonic and cyclic injection protocols designed to represent fault-valve cycles. We quantify how permeability evolves before, during, and after reactivation, and we explore the influence of key controlling factors: (i) initial permeability, (ii) initial stress state prior to injection, and (iii) confining stress. We also estimate seismic moments associated with individual reactivation events where the recovered moments remain bounded by the injected-volume constraint M0,max =GΔV  (McGarr, 2014). Overall, by adding grain-scale observations to trends reported in laboratory and in situ studies, this work helps interpret permeability transients and their implications for triggered seismicity, in order to provide more realistic models of fluid-induced fault reactivation.

References
Nguyen, H. N. G., Scholtès, L., Guglielmi, Y., Donzé, F. V., Ouraga, Z., & Souley, M. (2021). Micromechanics of sheared granular layers activated by fluid pressurization. Geophysical Research Letters. https://doi.org/10.1029/2021GL093222
McGarr, A. (2014). Maximum magnitude earthquakes induced by fluid injection. Journal of Geophysical Research: Solid Earth, 119, 1008–1019. https://doi.org/10.1002/2013JB010597

How to cite: Larkem, O., Scholtès, L., and Golfier, F.: A Multi-Scale Approach to Fault-Valve Systems and Their Evolution, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6001, https://doi.org/10.5194/egusphere-egu26-6001, 2026.

EGU26-6574 | ECS | Orals | EMRP1.3

Filling a missing piece of the 1855 Wairarapa earthquake: Rupture characteristics and implications for regional seismic hazard 

Duo Li, Andrew Howell, Genevieve Coffey, Kate Clark, Nicola Litchfield, Rob Langridge, Emmanuel Caballero Leyva, Rafael Benites, Charles Williams, Sanjay Bora, and Matt Gerstenberger

How large earthquakes rupture across mechanically distinct fault systems remains a fundamental unresolved problem in seismology. New Zealand straddles the Australia–Pacific plate boundary, where relative plate motion is partitioned between deep Hikurangi subduction and widespread dextral strike-slip faulting in the upper plate, such as the Marlborough Fault System. This tectonic configuration favours complex, multi-fault earthquakes, as illustrated by the 2016 Mw 7.8 Kaikōura earthquake and the 2013 Mw 6.5 and Mw 6.6 Cook Strait sequence in central New Zealand. Investigating the source physics of such complex ruptures and their relationship to plate-boundary architecture will provide essential constraints on fault interaction processes and seismic hazard in large-scale convergent margins.

On the evening of 23 January 1855, a major earthquake struck central New Zealand with intense ground shaking across much of the North and South Island. Empirical ground intensity was estimated up to ten, and local tsunami waves reached nearly 10 m in the Cook Strait (Grapes and Downes, 1997; Clark et al., 2019). This event is remarkable for having generated significant uplift - maximum uplift of 6.4 m measured in the southern Wellington coast (McSaveney et al., 2006) - and extreme dextral slip, measured as ~18.7 m at Pigeon Bush along the Wairarapa fault (Rodgers and Little, 2006).  Seismological evidence suggests an offshore hypocentre at ~25 km depth and a magnitude exceeding 8.0; however, in the absence of instrumental observations, it remains unclear whether significant slip also occurred on the Hikurangi subduction interface  (Beavan & Darby, 2005). Resolving the role of the deeper Hikurangi megathrust, particularly its potential synchronous activation with upper-plate faults, is therefore crucial for understanding the rupture mechanics of this event and for improving seismic hazard assessments in densely populated plate-boundary regions.

In this study, we investigate the source complexity and associated ground motions of multi-fault earthquakes using physics-based dynamic rupture simulations of the 2016 Kaikōura and 1855 Wairarapa earthquakes in central New Zealand. We construct dynamic source models accounting for updated geological and seismological constraints, including regional tectonic stress fields (Townend et al., 2012), national fault networks (Seebeck et al., 2024), nonlinear rheology, and three-dimensional subsurface structures. These key geophysical constraints are essential in reproducing the instrumental observations in the case of the 2016 Kaikōura earthquake (e.g. Ulrich et al. 2019).  Rupture magnitude and ground shaking of historical earthquakes are validated against geological measurements, landslide inventories, and tsunami run-up. Beyond observation-driven scenarios, we systematically explore the sensitivity of rupture dynamics and ground motions to variations in tectonic conditions in historical earthquakes. These simulations will provide physical constraints on rupture kinematics and fault interactions, offering insights into improving near-source ground-motion models and regional seismic hazard assessments.

How to cite: Li, D., Howell, A., Coffey, G., Clark, K., Litchfield, N., Langridge, R., Caballero Leyva, E., Benites, R., Williams, C., Bora, S., and Gerstenberger, M.: Filling a missing piece of the 1855 Wairarapa earthquake: Rupture characteristics and implications for regional seismic hazard, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6574, https://doi.org/10.5194/egusphere-egu26-6574, 2026.

The Gutenberg-Richter law for the distribution of earthquake magnitude and the Omori law for the decay of aftershocks are two universal laws in seismicity. Although numerical models have been developed to reproduce these laws, they sometimes produce many more foreshocks and less aftershocks than observed. In this study, we simulate earthquake sequences on a 2D random fault network. The fault lengths follow a power-law distribution. Our simulations reproduce the Omori law, without producing many foreshocks. The event size distribution follows Gutenberg-Richter's law with the b-value expected from the fault length distribution, even though many earthquakes are multi-fault ruptures or partial ruptures. Ruptures sometimes propagate into other faults, though there are more partial ruptures than multi-fault ruptures. The frequency of partial and cascading ruptures increases with higher fault density or stronger velocity-weakening friction. Overall, this work illuminates how fault interaction controls the spatiotemporal pattern of seismicity.

How to cite: Ozawa, S.: Partial ruptures, cascading multi-fault ruptures, and aftershocks in 2D random fault network, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8601, https://doi.org/10.5194/egusphere-egu26-8601, 2026.

EGU26-8994 | Posters on site | EMRP1.3

Rupture termination controlled by tuned stress heterogeneity on a 6-m-long laboratory rock fault 

Futoshi Yamashita, Eiichi Fukuyama, Kurama Okubo, and Yoshiaki Matsumoto

Understanding where and how rupture terminates on a fault is crucial because it controls earthquake magnitude and associated damage. But the in situ stress state, which is one of the key parameters governing rupture dynamics, is not directly measurable on natural faults. Laboratory experiments therefore provide an essential approach for investigating rupture termination (e.g., Bayart et al., 2016, 2018; Ke et al., 2018). Previous studies showed that termination can often be interpreted using an energy balance at the rupture tip within linear elastic fracture mechanics (LEFM), while also suggesting that incorporating additional processes such as long-tailed weakening or rate-dependent friction may improve the description (e.g., Paglialunga et al., 2022; Brener and Bouchbinder, 2021). In order to deepen our understanding of rupture dynamics, including how they terminate, it should be efficient to conduct a systematic investigation that controls the stress state and resulting rupture behavior in the laboratory. From this point of view, we have started a large-scale rock friction experiment. In our experiments, two metagabbro specimens are stacked vertically within the experimental frame. The contacting nominal area is 6.0 m long by 0.5 m wide. Six hydraulic jacks apply normal load to the upper block, and a single hydraulic jack applies shear load to the lower block, which is supported on low-friction rollers. Strain gauge arrays along the fault measure local shear stress every 130 mm at a sampling rate of 1 MHz. In experiment GB01-051, we first imposed 5 mm of shear displacement under a macroscopic normal stress of 2.8 MPa, generating repeated stick-slip events that nucleated at either the leading or trailing edge. We then gradually reduced the normal load on one of the normal jacks on the trailing-edge side while maintaining the shear load. This procedure produced clear nucleation near the unloaded jack followed by a full rupture across the entire fault. After restoring the loads to near-critical conditions, we repeated the procedure at the leading-edge side to generate fault ruptures. In a subsequent trailing-edge attempt, however, rupture terminated approximately halfway along the fault, despite a similar macroscopic stress level. Local stress measurements indicate that previous ruptures reduced the shear stress on the leading-edge side, lowering the available energy release rate for propagation and promoting termination. These results demonstrate that rupture initiation and termination can be manipulated through the evolving stress heterogeneity. We also estimated a lower bound on fracture energy from the measured stress drop using LEFM. Accounting for uncertainty in the termination location, the inferred value ranges from 0.032 to 0.29 J/m², consistent with prior experiments on the same rock type (Xu et al., 2019). Ongoing work will further quantify how controlled stress heterogeneity governs rupture termination.

How to cite: Yamashita, F., Fukuyama, E., Okubo, K., and Matsumoto, Y.: Rupture termination controlled by tuned stress heterogeneity on a 6-m-long laboratory rock fault, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8994, https://doi.org/10.5194/egusphere-egu26-8994, 2026.

The critical nucleation length (Lc) is a fundamental parameter that characterizes the earthquake nucleation process and is theoretically proportional to the fracture energy and the inverse square of shear stress drop (Andrews, 1976, JGR). However, quantitative verification of this relationship has been limited due to difficulties in controlling the nucleation location and in achieving spatially dense measurements capable of resolving the nucleation extent and associated stress drop on the fault.

In this study, we conducted large-scale rock-friction experiments using the biaxial friction apparatus to investigate the scaling characteristics of the critical nucleation length Lc. The experimental configuration consists of vertically stacked Indian metagabbro blocks, comprising an upper block (L6.0 m × W0.5 m × H0.75 m ) and a lower block (L7.5 m × W0.5 m × H0.75 m ), forming a simulated fault with a nominal contact area of 6.0 m × 0.5 m. Strain gauges were installed at a distance of 15 mm from the fault surface with a spacing of 130 mm, and continuous measurements were recorded at a sampling rate of 1 MHz. Normal loading was applied using six independently controlled jacks, enabling controlled rupture nucleation confined within the fault and high-resolution measurements of local shear-stress time history.

To establish a robust measurement criterion for Lc based on rupture velocity evolution, we performed 2D dynamic rupture simulations using spectral boundary integral equation software UGUCA (Kammer et al., 2021) with a linear slip-weakening law. We compared the theoretical Lc predicted from the frictional parameters and prescribed initial stress with Lc inferred from rupture-velocity-based criteria. By varying the critical slip distance Dc, we simulated nucleation processes with different Lc values. The results show that the preslip extent at which the rupture velocity reaches approximately 0.06Vs (where Vs is shear-wave velocity) is in good agreement with the theoretically predicted Lc, supporting the use of this criterion for quantifying and discussing the scaling of Lc.

Applying this criterion to the laboratory experiments, the estimated Lc values range from 0.4 m to 4.0 m, spanning nearly one order of magnitude. The average local shear stress drop within the estimated nucleation region was evaluated as the difference between the initial and residual shear stresses measured before and after the main shock. We observed that Lc clearly scales with the inverse of the shear stress drop, rather than the inverse square, which persists under different normal stress conditions. This scaling is consistent with the observation that the initial shear stress is close to the peak strength in the nucleation region, under the assumption that Dc remains nearly constant among events (approximately 1 μm in this study). These findings provide insight into the quantitative dependence of Lc on the shear stress drop and place important constraints on our understanding of earthquake nucleation processes.

How to cite: Matsumoto, Y., Okubo, K., Yamashita, F., and Fukuyama, E.: Earthquake Source Processes inferred from a 6-meter-long laboratory fault (1) Quantitative Evaluation of Critical Nucleation Length under Variable Stress Drops, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9293, https://doi.org/10.5194/egusphere-egu26-9293, 2026.

EGU26-9616 | Posters on site | EMRP1.3

Micromechanical Investigation of Fault-Valving Cycles Using the Discrete Element Method 

Luc Scholtès, Oussama Larkem, and Fabrice Golfier

Fault zones play a fundamental role in controlling subsurface fluid circulation and mineralization. Their capacity to alternately behave as barriers or conduits—commonly conceptualized within the fault-valve model—results from complex interactions among multiphysical processes (thermal, hydraulic, mechanical, and chemical) acting across a wide range of spatial and temporal scales within the fault structure.

Focusing on the gouge scale, we investigate the hydromechanical behavior of faults using a three-dimensional pore-scale modeling framework that couples a Discrete Element Method (DEM) with a pore-scale finite volume (PFV) scheme. Building on the approach of Nguyen et al. (2021), the DEM is used to model the gouge material as a granular assembly, while the PFV method is used to model fluid flow within the evolving pore space.

Using this coupled approach, we simulate a sheared, fluid-saturated granular gouge subjected to hydromechanical loading through a controlled cyclic fluid injection protocol applied at constant shear stress. The DEM-PFV model captures emergent behaviors consistent with laboratory and in situ observations, and reveals pronounced cycle-to-cycle variability in both the onset of reactivation (Sarma et al., 2025) and the magnitude of slip under repeated pressurization and depressurization. In particular, some cycles produce large slip episodes whereas others exhibit comparatively small slip under similar loading conditions. To connect this macroscopic variability to micromechanics, we track the evolution of the force-chain population throughout the cycles using the characterization method proposed by Peters et al. (2005). The results provide grain-scale insights into how internal load-bearing structures reorganize across cycles and how these force-chain dynamics relate to the occurrence of large-slip events in fault-valving sequences.

References
Nguyen, H. N. G., Scholtès, L., Guglielmi, Y., Donzé, F. V., Ouraga, Z., & Souley, M. (2021). Micromechanics of sheared granular layers activated by fluid pressurization. Geophysical Research Letters. https://doi.org/10.1029/2021GL093222
Sarma, P., Aharonov, E., Toussaint, R., & Parez, S. (2025). Fault gouge failure induced by fluid injection: Hysteresis, delay and shear-strengthening. Journal of Geophysical Research: Solid Earth. https://doi.org/10.1029/2024JB030768
Peters, J., Muthuswamy, M., Wibowo, J., & Tordesillas, A. (2005). Characterization of force chains in granular material. Physical Review E. https://doi.org/10.1103/PhysRevE.72.041307

How to cite: Scholtès, L., Larkem, O., and Golfier, F.: Micromechanical Investigation of Fault-Valving Cycles Using the Discrete Element Method, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9616, https://doi.org/10.5194/egusphere-egu26-9616, 2026.

EGU26-9839 | ECS | Posters on site | EMRP1.3

From thermal pressurization (TP) to dilatant strengthening (DS) during stick-slip ruptures on saturated saw-cut thermally cracked westerly granite 

Caiyuan Fan, Gang Lin, Jérôme Aubry, Damien Deldicque, Carolina Giorgetti, Harsha S. Bhat, and Alexandre Schubnel

In fluid-rich faults, thermal pressurization (TP) is theoretically predicted to induce rapid fault weakening and facilitate large earthquakes, whereas dilatant strengthening (DS) can counteract this process through pore-space expansion. This study experimentally investigates the relative efficiency and condition of TP and DS using triaxial stick-slip tests with on-fault pore pressure (Pp) measurements. Dynamic stick-slip events were generated on four saturated, saw-cut, thermally cracked Westerly granite samples under varying effective confining (30–60 MPa) and pore pressures (25–45 MPa). Results reveal a systematic rupture transition from co-seismic Pp rise (TP-type) at low shear stress to Pp drop (DS-type) at higher shear stress, accompanied by a coupled fast–slow spectrum: fast TP → slow TP → slow DS → fast DS. Fast events reach slip velocities up to three orders of magnitude higher (0.5–10 mm s-¹) than slow ones (0.001–0.5 mm s-¹). The TP model under undrained, adiabatic conditions reproduces the measured Pp evolution, indicating a progressive shear-zone widening (0.05–0.5 mm, as overestimated values) that reduces TP efficiency and promotes slow events. For DS sequences, an increasing dilatancy coefficient is inferred, consistent with enhanced Pp drops. Breakdown energy shows no clear difference between TP and DS events, suggesting similar rupture energetics despite opposite pore-pressure evolution. Overall, this study provides the first direct experimental evidence of TP–DS transitions, demonstrating that TP governs early-stage weakening but diminishes as the shear zone widens, allowing DS to dominate. These results imply that in mature fault zones, after several seismic cycles, fault weakening may be mainly governed by co-seismic dilatancy, although strong, fast ruptures can still occur when the dilatant strengthening is not sufficient to stop the on-going rupture.

How to cite: Fan, C., Lin, G., Aubry, J., Deldicque, D., Giorgetti, C., S. Bhat, H., and Schubnel, A.: From thermal pressurization (TP) to dilatant strengthening (DS) during stick-slip ruptures on saturated saw-cut thermally cracked westerly granite, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9839, https://doi.org/10.5194/egusphere-egu26-9839, 2026.

EGU26-12207 | ECS | Orals | EMRP1.3

Can Earthquake magnitude be predicted at rupture onset? insights from scaled seismotectonic models 

Silvio Pardo, Fabio Corbi, Simona Guastamacchia, Giacomo Mastella, Elisa Tinti, and Francesca Funiciello

The largest earthquakes on planet Earth occurred along the frictional interface between subducting and overriding plates (i.e., the megathrust) at convergent margins. Some of these destructive events have occurred over the last 20 years, such as the 2004 Mw 9.0 Sumatra‐Andaman, 2010 Mw 8.8 Maule, and 2011 Mw 9.0 Tōhoku‐Oki earthquakes. These large events are among the most devastating expressions of Earth's dynamics and, along with tsunamis, they represent a major hazard to society. Therefore, it is crucial to understand to which extent it is possible to predict the final size of a large rupture from the early stage of its propagation. We studied analog earthquakes in an apparatus - Foamquake (Mastella et al., 2022) - in which we used foam rubber to reproduce the upper plate and a 1 cm thick layer of granular materials to reproduce the subduction channel. The set-up is made of an elastic foam wedge with a dimension of 145 × 90 × 20 cm3 (i.e., the overriding plate analog) that overlies a planar, 10° dipping, rigid plate. Along the plate, a basal conveyor belt is driven with constant velocity (0.01 cm/s), reproducing a steady, trench-orthogonal subduction. To constrain the dynamics of analog earthquakes, we used a network of 11 Micro-Electro-Mechanical Systems (MEMS) accelerometers, distributed on the model surface, and measured the evolution of the trench orthogonal component of acceleration at 1 kHz. Additionally, we also used a top-view high-resolution camera (100 Hz), that allows us to derive surface displacements via Particle Image Velocimetry (PIV), that enables characterization of the final static rupture properties, while MEMS monitoring resolves the temporal evolution of spatiotemporal slip. We report 21 models with different frictional configurations of the analog megathrust, including asperities and barriers of varying dimensions, to produce thousands of events with different magnitudes. MEMS monitoring allows for characterization of the Source Time Function (STF) of each event. Preliminary analysis of the STFs indicates a weak correlation  (i.e., R2<0.2) between the moment accumulated over different time windows during the early stages of rupture propagation and the final size of individual events. These results contribute, from an experimental perspective, to the ongoing debate on the stochastic versus deterministic nature of earthquake rupture growth.

How to cite: Pardo, S., Corbi, F., Guastamacchia, S., Mastella, G., Tinti, E., and Funiciello, F.: Can Earthquake magnitude be predicted at rupture onset? insights from scaled seismotectonic models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12207, https://doi.org/10.5194/egusphere-egu26-12207, 2026.

EGU26-12872 | ECS | Orals | EMRP1.3

Fluid-assisted frictional healing revealed by ultrasonic waves 

Michele Mauro, Giovanni Guglielmi, Fabio Trippetta, and Marco Scuderi

The seismic potential of a fault is controlled by its ability to regain strength between earthquakes (fault healing). Variations in healing rate among different rock types can cause local locking and elastic strain energy accumulation, potentially leading to earthquake nucleation. The 2016 Mw 6.5 Norcia mainshock nucleated in the Triassic Evaporites, the seismogenic layer of central Italy, composed of dolostones and anhydrites. Despite its relevance, the mechanical behavior of anhydrite remains relatively less constrained compared to other common crustal lithologies. Only a limited number of studies have systematically investigated the frictional properties of anhydrite, suggesting that its mechanical behavior is strongly sensitive to boundary conditions.

We conducted room humidity (RH) and water-saturated (WS) Slide-Hold-Slide (SHS) friction experiments on anhydrite gouge to assess and isolate the role of water on its healing properties. To inform mechanical data with the microphysical evolution of the fault, we used piezoelectric (PZT) sensors in transmission mode, which record ultrasonic S-wave (UW) propagation through the sample. Finally, mechanical and ultrasonic measurements were complemented by microstructural analyses of the post-mortem sample.

Our results show that fault healing follows a log-linear dependence on hold time under both RH and WS conditions, but with markedly different magnitudes. Water-saturated experiments exhibit a healing rate nearly three times larger (β ~ 0.024) than RH experiments (β ~ 0.009). Ultrasonic measurements reveal a systematic log-linear increase in S-wave velocity during hold periods. This growth is significantly more pronounced in WS samples, where S-wave velocity increases by more than ~2.8% per decade of hold time, compared to ~1% in RH conditions. Microstructural observations indicate that RH samples deform through distributed cataclastic processes accommodated by multiple R-shear bands, whereas WS samples exhibit extreme strain localization along B-shear zones characterized by intense grain-size reduction and the development of a compressive foliation, consistent with semi-brittle deformation.

These results demonstrate that water fundamentally alters the healing efficiency and deformation style of anhydrite faults. Moreover, they show that ultrasonic wave measurements provide a powerful, independent tool to track fault restrengthening during simulated interseismic periods. The observed increase in S-wave velocity can be directly linked to an increase in the shear modulus of the gouge, which appears to be greater in the presence of water, probably due to fluid-assisted healing processes. Together, the high healing rates and the mechanical stiffening of the microstructure inferred from S-wave velocity measurements suggest that anhydrite gouge may be capable of efficiently accumulating elastic strain energy during interseismic periods. Our findings suggest that fluid-assisted healing in anhydrite-bearing fault zones may play a critical role in controlling fault stability and seismic behavior in natural settings.

How to cite: Mauro, M., Guglielmi, G., Trippetta, F., and Scuderi, M.: Fluid-assisted frictional healing revealed by ultrasonic waves, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12872, https://doi.org/10.5194/egusphere-egu26-12872, 2026.

In laboratory studies, the tendency for earthquake nucleation on major plate-boundary fault zones is typically evaluated by measuring the change in shear strength upon controlled step changes in driving velocity.  In such laboratory shear experiments simulating fault sliding, it is typical to neglect the cohesion and assume that all the measured shear strength is due to frictional resistance.  Therefore, the results of such experiments are evaluated in terms of a friction coefficient calculated as the ratio of the shear strength to effective normal stress, where the “velocity-dependent friction” is quantified by the parameter a-b.  However, previous work has shown that the sliding cohesion is not necessarily negligible, especially for water-saturated samples rich in clay-minerals.  This comes from recent experiments have shown that, using a single-direct type shear geometry, the cohesion can be directly measured as a peak shear strength with zero applied normal load (zero effective normal stress).  The technique can also be used for samples that have accumulated slip, thus providing a measure of the cohesion that exists during sliding or “sliding cohesion”.

Here, I use measurements of sliding cohesion to test the assumption that velocity-dependent fault strength is completely controlled by friction, and determine if cohesion plays a significant role.  For these tests I use water-saturated powdered illite-rich Rochester shale, a material that consistently exhibits velocity-strengthening behavior.  The velocity-dependent strength is first obtained with a series of standard 3-fold step increases in driving velocity in the range 0.1-100 μm/s under 10 MPa effective normal stress.  The sliding cohesion is then measured in a series of experiments in which the samples were sheared for 5 mm under 10 MPa effective stress, the normal stress subsequently removed, and then sheared at each of the velocities used in the velocity-step test.  From these tests, the velocity-dependent cohesion is calculated by substituting the cohesion for shear strength and calculating an equivalent “a-b” value that can be subtracted from the standard a-b value measured from the velocity step tests. 

Preliminary results show that velocity-dependent cohesion is of the same order as a-b values, and accounts for up to about a third of the measured a-b values.  The percentage of strength change related to cohesion rather than friction decreases as a function of increasing driving velocity.  Although cohesion is a significant proportion of the velocity-dependent strength changes, removing the velocity-dependence of cohesion is insufficient to cause negative a-b values.  However, this result can also be affected by the choice parameters used in the modeling technique that extracts the a-b values and must therefore be evaluated carefully.  The magnitude of velocity-dependent cohesion suggests that it may represent a signification proportion of velocity-dependent sliding strength.

How to cite: Ikari, M.: Considering velocity-dependent cohesion in fault sliding stability, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14228, https://doi.org/10.5194/egusphere-egu26-14228, 2026.

EGU26-14469 | Posters on site | EMRP1.3

Earthquake Source Processes inferred from a 6-meter-long laboratory fault (2): Fracture Energy Estimation from Dynamic Stress Fields 

Kurama Okubo, Futoshi Yamashita, Yoshiaki Matsumoto, and Eiichi Fukuyama

Fracture energy is a key scaling parameter governing the transition from quasi-static nucleation to dynamic rupture propagation, and it also controls the dynamic stress field around the rupture front. In principle, when fracture energy is uniform along a fault, a single intrinsic fracture energy should describe both quasi-static nucleation and the stress field during rupture propagation. However, this unifying role has not been fully validated experimentally, primarily because conventional laboratory faults are too small to capture the entire rupture process from nucleation to propagation toward limiting speed. Here, we compare the fracture energy evaluated from the shear stress changes associated with the dynamic rupture propagation (Γ) with that inferred from the independently observed critical nucleation length (GLc) on a 6-meter-long laboratory fault.

We conduct faulting experiments on a 6-meter-long laboratory fault and evaluate fracture energy by fitting a steady-state rupture model with a linear cohesive zone to local shear stress changes recorded 15 mm away from the fault. In the biaxial rock-friction apparatus, vertically stacked rock specimens form a simulated fault with dimensions of 6 m × 0.5 m. Six independently controlled jacks applying normal loading enable rupture nucleation at prescribed timing and location by unloading a selected jack while maintaining the shear stress near the peak frictional strength. Rupture velocity is constrained by cross-correlating shear stress histories between neighboring strain gauges spaced at 130 mm. Using the locally estimated rupture velocity, fracture energy Γ and cohesive zone size are determined by minimizing the residual between observed and modeled shear stress time histories.

Fracture energy inferred from critical nucleation length, GLc, is computed following the formulation of Palmer and Rice (1973) and Andrews (1976), using the critical nucleation length examined by Matsumoto et al. (2026, EGU) togather with the measured stress drops.

We analyze three nucleation-controlled events conducted under a macroscopic normal stress of 3 MPa. From local shear stress time histories associated with rupture velocities lower than 0.95 of the Rayleigh wave speed, we obtained an average fracture energy Γ of 0.04 ± 0.01 J/m². This value is consistent with GLc of 0.05 J/m², inferred from events with an average stress drop of 0.05 MPa. These results contribute to the quantitative interpretation of laboratory observations and to improved understanding of earthquake source processes on natural faults.

How to cite: Okubo, K., Yamashita, F., Matsumoto, Y., and Fukuyama, E.: Earthquake Source Processes inferred from a 6-meter-long laboratory fault (2): Fracture Energy Estimation from Dynamic Stress Fields, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14469, https://doi.org/10.5194/egusphere-egu26-14469, 2026.

EGU26-14558 | Orals | EMRP1.3

Heterogeneous Stress–Driven Shear Localization Governing Fault Slip in Decimeter-Scale Quartz Gouge under Variable Surrounding Stiffness 

Giacomo Mastella, Giuseppe Volpe, Martijn Van den Ende, Michele De Solda, Fabio Corbi, Francesca Funciciello, Chris Marone, and Scuderi Marco

Fault slip stability is governed by the competition between the elastic energy stored in the surrounding medium and the rate of frictional weakening of the fault, which depends on its constitutive frictional properties. Laboratory shear experiments validate this framework under simplified conditions and homogeneous boundary conditions. In contrast, natural faults are heterogeneous across multiple scales, with variations in stress, frictional properties, fault-zone structure, and elastic properties as documented in laboratory, numerical, and field studies. In gouge-filled faults,  heterogeneities are dynamically coupled: stress concentrations promote shear localization, which modifies gouge fabric that controls the frictional properties, ultimately dictating fault stability and rupture dynamics. Resolving how spatially heterogeneous stress and evolving fault-zone structure interact to control rupture nucleation and propagation therefore requires experimental approaches that move beyond homogeneous assumptions.

Here we present results from large-scale biaxial shear experiments on a quartz gouge–filled fault (75 cm × 8 cm) using two forcing-block materials—Nylon 6 and PMMA—with different elastic stiffnesses. The fault was densely instrumented to investigate how stress heterogeneity and evolving shear fabric control slip behavior under different nominal normal stresses from 3 to 10 MPa and a constant loading rate of 10 µm/s. Far-field stress and displacement were monitored using load cells and LVDTs (1 kHz), while forcing blocks deformation was measured using Digital Image Correlation (DIC, 2–30 Hz). During laboratory earthquakes, local fault slip and volumetric deformation were recorded using eddy-current displacement sensors (1.25 MHz) and high-speed DIC (10 kHz). Emitted acoustic waves were recorded at 3.125 MHz using an array of 33 piezoelectric sensors calibrated through ball-drop tests, active-ultrasonic survey, laser vibrometry, and spectral-element waveform modeling.

The experiments produce a broad spectrum of slip behaviors, from stable creep, slow ruptures to fast, dynamic events. Transitions from slow to fast slip are promoted by increasing normal stress and decreasing elastic stiffness. Co-seismic slip, peak slip velocity, and high-frequency acoustic energy increase systematically with cumulative fault slip, increasing normal stress, and decreasing loading stiffness. Direct measurements of slip enable estimation of the critical nucleation length, which decreases with increasing cumulative slip and normal stress, in agreement with theoretical predictions. Finite-element modeling shows that the experimental geometry induces heterogeneous stress distributions promoting the development of heterogeneous shear fabrics and spatially variable frictional responses. When shear fabric is well developed, normal stress is low, and the nucleation lengths are correspondingly large, stress heterogeneities have little impact  on slip dynamics, which is dominated by system spanning events with regular, periodic seismic cycles. Conversely, at higher normal stress—conditions associated with smaller nucleation lengths—and/or poorly developed shear fabric, stress heterogeneity drives complex slip behavior, including partial and full ruptures and rupture cascades characterized by strongly spatially variable stress drops. These results highlight how the coupled evolution of stress, shear fabric, and frictional heterogeneities controls slip dynamics in gouge-filled faults.



How to cite: Mastella, G., Volpe, G., Van den Ende, M., De Solda, M., Corbi, F., Funciciello, F., Marone, C., and Marco, S.: Heterogeneous Stress–Driven Shear Localization Governing Fault Slip in Decimeter-Scale Quartz Gouge under Variable Surrounding Stiffness, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14558, https://doi.org/10.5194/egusphere-egu26-14558, 2026.

EGU26-15062 | ECS | Orals | EMRP1.3

Bridging inner fault shear localisation and the propagation of earthquake rupture 

Fabian Barras and Nicolas Brantut
Earthquakes leave different types of records that help decipher their dynamics. At the large scale monitored by remote sensing and seismic data, earthquakes arise from the propagation of rapid slip along tectonic faults, exhibiting rupture dynamics reminiscent of those driving shear fracture or slip fronts in stick-slip experiments. At the scale of the fault core, fieldwork revealed how the zone actively deformed during an earthquake is often extremely thin and that shear strains are highly localised.
In this work, we numerically simulate shear ruptures using a dual-scale approach, allowing us to couple a sub-millimetre description of inner fault processes and kilometre‑scale elastodynamics. Our results demonstrate how rapid strain localisation across a layer of fault gouge creates a sudden drop in the shear stress bearing capacity, producing earthquake rupture that closely follows fracture mechanics description. We quantify how the fracture energy governing rupture propagation is substantially smaller than that predicted by models that do not account for strain localisation. We show the existence of a unique scaling law between the localised shearing width and the rupture speed. Our results bring new insights on the multiscale mechanics that produces seismic rupture and indicate that earthquakes are likely to be systematically associated to extreme strain localisation.

How to cite: Barras, F. and Brantut, N.: Bridging inner fault shear localisation and the propagation of earthquake rupture, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15062, https://doi.org/10.5194/egusphere-egu26-15062, 2026.

Earthquakes represent the most visible manifestation of tectonic stress accumulation and release within the Earth’s lithosphere. Despite their fundamental importance, the absolute stress levels that drive earthquake rupture remain poorly constrained. In particular, fault shear strength is strongly influenced by fluid pressure at depth, yet its magnitude and variability, especially within the locked zones of megathrusts and across different tectonic regimes, are still not well understood. In this study, I estimate the shear strength of the lithosphere by quantifying the total energy budget of large earthquake ruptures. The total released energy is partitioned into radiated energy and energy dissipated during fault slip, commonly referred to as breakdown (or fracture) energy (G). Radiated energy can be robustly estimated from seismic waveforms or earthquake source time functions. In contrast, reliable estimates of fracture energy are more challenging. To address this, I employ a finite-width slip-pulse model for steady-state dynamic rupture propagation (Rice et al., 2005), combined with heterogeneous kinematic rupture models of large earthquakes. The analysis is based on 208 finite-fault rupture models from the NEIC database, spanning Mw ≥ 7 earthquakes between 1990 and 2025. The adoption of a self-healing pulse rupture framework is motivated by the widely observed property that earthquake rise times are approximately an order of magnitude shorter than total rupture durations, on average about one-seventh of the rupture time in my database.

My results indicate that fracture energy (G) is strongly controlled by the heterogeneous distribution of rupture velocity, rise time, and slip during earthquake rupture. Fracture energy is underestimated by approximately a factor of five when heterogeneity in the rupture process of large earthquakes is neglected, and by nearly an order of magnitude when estimates are based on a classical crack rupture model. Assuming that megathrust earthquakes undergo an almost complete strength drop during rupture, as observed for the 2011 Tohoku earthquake, our estimates represent lower bounds on fault shear strength across global subduction zones and the oceanic lithosphere. The results reveal pronounced fault weakening during megathrust ruptures, with a global average shear strength of approximately 6 MPa. Tsunami earthquakes correspond to the weakest faults, with shear strengths on the order of ~2 MPa, implying that fluid pressures are extremely elevated across most subduction interfaces worldwide. Using these shear strength estimates, I infer a global average pore-fluid pressure ratio (λ = Pf / σlith) of approximately 0.9 for subduction megathrusts. In contrast, the oceanic lithosphere at mid-ocean ridges, transform faults, and fracture zones is nearly an order of magnitude stronger, indicating fluid pressures close to hydrostatic conditions. These pronounced contrasts demonstrate that fluid pressure may play a first-order role in controlling the strength of the Earth’s lithosphere.

How to cite: Pulido, N.: Estimation of fault fracture energy and shear strength drop in large earthquakes: Implications for fluid pressure and tectonic regime, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16466, https://doi.org/10.5194/egusphere-egu26-16466, 2026.

EGU26-16867 | ECS | Posters on site | EMRP1.3

Microstructural and Frictional Consequences of Slip Velocity Variations: Insights from a single-asperity lab-fault experiment 

Adriane Clerc, Guilhem Mollon, Amandine Ferrieux, Lionel Lafarge, and Aurélien Saulot

Understanding earthquakes mechanisms still represents a challenge. The complexity of both the fault zone and the fault behaviour requires to make some simplifications and to downscale the studied system.

 In our work, we aim at creating a down-scaled experimental fault model where the behaviour of the asperities and the shearing of the granular gouge are both considered. In order to do so, we borrow from the tribological approach the pin-on-disk experiment: the original experimental apparatus consists in a centimetric pin with a hemispherical extremity representing the fault asperity while a large flat rotating disk stands for the opposite surface of the experimental fault. Both parts are made in the same carbonate rock with controlled roughness. Co-seismic conditions (Velocity in the range [0.001 – 1]  m/s, Normal stress in the range [4 – 400] MPa) are applied during the different experimental tests. A number of high-sampling-rate sensors are used to constrain the observation of the asperity-track contact during the simulated seismic events. Moreover, complete post-mortem analyses of the contact surfaces allow to quantify the mechanisms and to reconstruct friction scenarios in accordance with the time-series acquired during tests.

In a previous work, we determined the conditions most representative for a mature lab-fault. In the present study, we focus on the changes in wear and friction behaviours in the lab-fault linked to the slip velocity variations and the presence of granular gouge. Wear is mostly dependent on the slip velocity and the granular gouge layer thickness obtained at the mature conditions appears as an optimal thickness to limit wear. Here, velocity weakening is observed, with dramatic consequences on the microstructure of the contact surfaces. SEM and optical images show evidences of the combination of high stresses and heating on the first layer of minerals of the contact zone.

How to cite: Clerc, A., Mollon, G., Ferrieux, A., Lafarge, L., and Saulot, A.: Microstructural and Frictional Consequences of Slip Velocity Variations: Insights from a single-asperity lab-fault experiment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16867, https://doi.org/10.5194/egusphere-egu26-16867, 2026.

EGU26-17231 | Posters on site | EMRP1.3

In-situ X-ray imaging of stick-slip behavior in small-scale polystyrene fault analogs 

Bastien Walter and Audrey Bonnelye

Understanding the mechanisms controlling fault slip requires dedicated experimental setups that bridge the gap between natural conditions and observable scales. These experiments may require the use of analogue materials adapted to the scale of the laboratory, which present interesting characteristics facilitating the observation of physical processes. Polystyrene, due to its low strength and elastic properties, and structure, offers an effective analog material to investigate mechanical fault processes at both large (metric) and small scales (cm). Its low elastic properties slows down deformation processes and enables in-situ small scale observations using X-ray microCT.

In this study, we performed uniaxial compression experiments on small polystyrene blocks with a pre-cut slip interface. Polystyrene of various initial densities were tested. Compression rates ranged from 0.1 to 1 mm/min to induce different slip modes, from slow slip to dynamic stick-slip events. Real-time 2D X-ray radiography was coupled with mechanical monitoring to capture the onset and evolution of slip along the interface. Additionally, 3D scans were acquired at various stages during compression, with the objective of evaluating the spatial distribution of deformation around the fault plane over time.

The aim of this study is to combine mechanical data and imaging in order to characterize internal density changes associated with deformation. Preliminary observations seem to highlight density contrasts in the bulk material around the fault plane, offering insight into potential precursory signs of slip.

This approach demonstrates the potential of X-ray microCT for high-resolution monitoring of analog fault models, with perspectives for quantifying strain localization and post-slip damage patterns. These results may contribute to the understanding of frictional behavior and rupture dynamics in scaled experiments.

How to cite: Walter, B. and Bonnelye, A.: In-situ X-ray imaging of stick-slip behavior in small-scale polystyrene fault analogs, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17231, https://doi.org/10.5194/egusphere-egu26-17231, 2026.

EGU26-17445 | ECS | Posters on site | EMRP1.3

Imaging and forecasting rupture dynamics of induced microearthquakes 

Nico Schliwa, Francesco Mosconi, Elisa Tinti, Aurora Lambiase, Katinka Tuinstra, Alice-Agnes Gabriel, Antonio Pio Rinaldi, Men-Andrin Meier, Massimo Cocco, and Domenico Giardini

Understanding the faulting dynamics of natural earthquakes is fundamentally limited by the scarcity of near-source observations and the incompleteness of knowledge about in situ conditions at depth. The Bedretto Underground Laboratory for Geosciences and Geoenergies (BedrettoLab) in Switzerland addresses these limitations through controlled hydraulic stimulation experiments that generate seismicity beneath more than 1 km of rock overburden, thereby bridging the scale gap between laboratory studies and observed natural earthquakes. A key advantage of the BedrettoLab is the ability to characterize in situ conditions prior to seismicity induction. This includes imaging the geometry of the target fault, estimating the local stress state and pore fluid pressure, and examining host and fault rock properties.

Seismicity induced by controlled hydraulic stimulation is recorded by a comprehensive suite of near-source instrumentation, including strong-motion seismometers, borehole geophones and accelerometers, high-frequency acoustic emission sensors, and fibre-optic cables enabling Distributed Acoustic Sensing (DAS) and Fibre Bragg Grating (FBG) measurements. Past experiments have successfully generated seismicity sequences with mainshock magnitudes between Mw −0.5 and 0.0. We construct dynamic rupture models for one such mainshock, constrained by the available near-source observations, to image slip distribution, rupture directivity, and rupture velocity at meter-scale resolution. We find that rupture directivity has a substantially stronger impact on spectral amplitudes than average stress drop. The inferred stress and friction drops are interpreted in terms of the maximum possible confining pressure, providing insights into dynamic weakening processes during earthquake rupture.

The next experiment aims to induce Mw 1.0 earthquakes along a selected fault zone. Using constraints from hydraulic fracture tests, fault geometry imaging, and injection protocols, we seek to forecast the potential rupture dynamics of the induced mainshock by generating a suite of dynamic rupture models representing plausible rupture scenarios, against which the observed mainshock dynamics can be evaluated. In particular, we assess how reliably pre-experiment slip tendency analyses translate into the actual rupture behavior under these controlled conditions. Ultimately, this research will advance our understanding of earthquake source physics and contribute to improved forecasting and mitigation of worst-case scenarios associated with hydraulic stimulation.

How to cite: Schliwa, N., Mosconi, F., Tinti, E., Lambiase, A., Tuinstra, K., Gabriel, A.-A., Rinaldi, A. P., Meier, M.-A., Cocco, M., and Giardini, D.: Imaging and forecasting rupture dynamics of induced microearthquakes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17445, https://doi.org/10.5194/egusphere-egu26-17445, 2026.

EGU26-17533 | ECS | Posters on site | EMRP1.3

P- and S-wave precursors to lab earthquakes under variable drainage and fluid pressurization 

Raphael Affinito, Pengliang Yu, Derek Elsworth, and Chris Marone

Fault slip emerges from coupled frictional and hydromechanical processes, yet forecasting stress evolution remains challenging when fluid pressurization, drainage, and dilatancy modulate effective normal stress. We present laboratory double-direct shear experiments on quartz-rich natural fault gouge conducted under dry, 100% humidity, and constant fluid-pressure boundary conditions. Throughout quasi-periodic and irregular seismic cycles, we continuously acquire active-source ultrasonic waveforms transmitted across the gouge layer and derive cycle-resolved acoustic observables: P- and S-wave velocity changes and amplitude-based transmissivity metrics (band-limited RMS).

For our range of conditions, the acoustic properties exhibit robust, two-stage precursory evolution. During the early interseismic phase, acoustic transmissivity increases with contact stress, consistent with progressive asperity contact growth and rising contact stiffness (“healing”). This is followed by a late interseismic-to-preseismic transition characterized by gradual bulk velocity reduction, interpreted as distributed inelastic creep and microcrack growth within the gouge. For the 100% humidity condition, velocity changes track slip velocity, peaking as the fault locks and decreasing prior to dynamic slip. Under constant external fluid pressure, partial drainage and localized undrained behavior further modulate both elastic velocity and transmissivity through shear-induced porosity changes and associated pore-pressure transients. Localized slip regions can show transient acoustic velocity increases consistent with dilatancy hardening, while the bulk response trends toward overall velocity decrease as failure approaches.

We develop a mechanistic poromechanical framework that links the ultrasonic observables to evolving contact stiffness, porosity, and effective stress, providing a physical basis for interpreting travel-time and amplitude changes under fluid pressurization. As an additional validation, a lightweight sequence model trained on the acoustic observables can reconstruct cycle-scale shear-stress evolution and event timing, demonstrating that the acoustic measurements encode the state of the fault. These results highlight the role of fault zone elastic properties for detection of precursory processes prior to earthquake failure and illuminate the processes that occur during the preparatory stages of earthquake nucleation for fluid-saturated fault systems.

How to cite: Affinito, R., Yu, P., Elsworth, D., and Marone, C.: P- and S-wave precursors to lab earthquakes under variable drainage and fluid pressurization, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17533, https://doi.org/10.5194/egusphere-egu26-17533, 2026.

EGU26-18859 | ECS | Posters on site | EMRP1.3

Complex interaction between brittle and ductile rheologies in slow laboratory earthquakes 

Giovanni Guglielmi, Michele Mauro, Marco Scuderi, Cristiano Collettini, and Fabio Trippetta

Earthquakes originate from frictional instabilities that nucleate and propagate along faults cutting through a multilayered crust. Geological observations show that fault zones are complex structures often composed of heterogeneous mineral assemblages with contrasting frictional rheologies, whose interaction strongly influences slip behavior during fault reactivation. Two major earthquakes (Mmax > 6) that struck central Italy in the past 30 years–the 1997 Colfiorito and 2016 Norcia events–nucleated within Triassic Evaporites (TE) consisting of anhydrites and dolostones. Previous laboratory experiments on stick-slipping faults in TE gouges highlighted the key role of shear zone fabric in controlling breakdown processes and slip dynamics. However, the individual contribution of each lithology to frictional failure mode remains unclear.

Here we present preliminary results from laboratory friction experiments on powdered TE samples aimed at disentangling the role of anhydrite and dolostone in controlling fault slip behavior and dynamics in TE faults. We conducted double-direct shear experiments on three gouge compositions: 100% anhydrite, 50:50 anhydrite-dolostone, and 100% dolostone. The experimental procedure comprises two main stages: (i) a fabric development phase, in which the gouge is sheared under 50 MPa normal stress at a load-point velocity of 10 μm/s; and (ii) a fault reactivation phase at boundary conditions designed to enhance frictional instabilities that are: normal stress reduced to 30 MPa, a low-stiffness element inserted in series with the shear loading axis, and re-shearing at 1 μm/s. We also monitored the evolution of the fault physical properties from fabric development to stick-slip, via an ultrasonic system that continuously transmits and receives acoustic waves through the experimental fault.

During the fabric development stage, all three fault gouges display stable sliding with a friction coefficient μ of ~ 0.6. In the fault reactivation stage, anhydrite faults exhibit slow (v < 20 μm/s), repetitive stick-slip with small stress drops (Δ𝛕 < 0.1 MPa), whereas dolostone faults accommodate shear through stable sliding. Interestingly, the 50:50 anhydrite-dolostone mixture does not exhibit intermediate behavior between the two  end-members but instead develops larger (0.1 < Δ𝛕 < 0.4 MPa), yet generally slower (v < 10 μm/s), slip instabilities, indicating a nonlinear mechanical interaction between anhydrite and dolostone.

Post-experiment microstructural analyses reveal that single-component gouges deform via cataclastic flow and frictional sliding along boundary and Riedel shear bands. In contrast, the 50:50 mixture exhibits extremely localized boundary shear planes dominated by nanometric dolostone particles embedded within foliated anhydrite-dolostone S-C structures. These features suggest a significant contribution of ductile, distributed deformation to energy dissipation during slow frictional ruptures. Ongoing ultrasonic wave analyses aim to characterize the relationship between the evolution of the elastic properties of the fault gouge, its internal structure, and the resulting slip behavior.

Our results provide new insights into the complex interplay between different frictional rheologies within fault zones of the seismogenic layer of northern Apennines, and highlight the role of compositional heterogeneity in controlling fault slip dynamics and energy dissipation.

How to cite: Guglielmi, G., Mauro, M., Scuderi, M., Collettini, C., and Trippetta, F.: Complex interaction between brittle and ductile rheologies in slow laboratory earthquakes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18859, https://doi.org/10.5194/egusphere-egu26-18859, 2026.

EGU26-22410 | Posters on site | EMRP1.3

Effect of long preexisting fractures on fault nucleation processes 

Taka Kanaya

The physics underlying earthquake precursory phenomena remains poorly constrained, particularly in crustal materials containing long preexisting fractures.  We conduct axial compression experiments on pre-heated Fontainebleau sandstone with acoustic emission (AE) monitoring under confining and pore pressures of 30 and 5 MPa, respectively.  Preliminary results show no systematic differences in precursory AE behavior between pre-heated and as-is samples.  All samples exhibit b values between 0 and 1, with a wide range of overall b-value evolution toward failure, including both increasing and decreasing trends.  Despite this variability, many samples show a local decrease in b value immediately before and during failure, preceded by a local increase near peak stress.  These local b-value variations likely reflect distinct microfracturing processes in porous granular rocks, contrasting with the more monotonic b-value decrease commonly reported for crystalline rocks.  Our results suggest that subtle differences in initial granular microstructure promote diverse precursory behavior under otherwise identical experimental conditions.  Such variability may contribute to the range of precursory behavior observed in tectonic earthquakes, where many large events are not preceded by a decrease in b value.  To investigate the role of aseismic deformation in fault nucleation, we are currently quantifying the evolution of microfracture distributions in deformed samples.  In parallel, we are deforming samples containing long preexisting fractures by first pre-deforming them in the semibrittle regime at higher pressure–temperature conditions, followed by deformation to failure at lower pressure–temperature conditions.  These experiments constrain the evolution of seismic and aseismic precursory signals toward large earthquakes in highly fractured crust.

How to cite: Kanaya, T.: Effect of long preexisting fractures on fault nucleation processes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22410, https://doi.org/10.5194/egusphere-egu26-22410, 2026.

EGU26-313 | ECS | Orals | EMRP1.6

Contact Stress Distribution and Slip Stability on Experimental Faults 

Julia Baumgarte, Lekima Yakuden, and James Kirkpatrick

The roughness of natural fault surfaces means that faults make contact at discrete, high-stress bumps and other geometrical highs, producing extreme spatial heterogeneity in normal stress on the sliding interface. This heterogeneity plays a crucial role in nucleating and arresting earthquake rupture. However, heterogeneity resulting from contact of rough surfaces has not been systematically tested in laboratory experiments, which have previously been restricted to nominally flat surfaces. We investigate how the spacing of macroscopic contact regions controls slip stability by shearing cement blocks designed and manufactured to have prescribed contact spacing, as well as replicas of a natural fault surface. Arrays of hemispherical bumps were manufactured with initial spacings of 22-235 mm. Experiments were conducted in direct shear at normal loads ranging from 1 to 10 kN, resulting in local contact stresses of ~20-120 MPa.

Across 27 experiments, sliding ranged from stable creep to unstable stick-slip behavior. Instability is controlled by the minimum spacing between adjacent contact regions (λc), which evolves during wear. Faults remain stable when λc is less than the critical nucleation length Lc predicted by fracture mechanics (tens to ~180 mm for our measured G, Dc, σ, and Δf). When λc exceeds Lc, stick-slip initiates regardless of overall friction coefficient or surface type (regular hemisphere arrays, random bumps, or natural fault replicas). Increased contact normal stress also promotes instability by reducing Lc. These findings are corroborated by a case study of a single experiment, in which λc increased abruptly upon the loss of a few individual contacts, resulting in the immediate transition from stable to unstable sliding that occurred precisely as λc crossed Lc, independent of changes in contact radius.

Our results demonstrate that the spacing of high-stress contact patches may significantly influence slip stability on faults. Because this spacing length scale can be directly observed on real fault surfaces, it provides a physically grounded predictor of where rupture can nucleate or arrest across scales from hand samples to fault segments.

How to cite: Baumgarte, J., Yakuden, L., and Kirkpatrick, J.: Contact Stress Distribution and Slip Stability on Experimental Faults, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-313, https://doi.org/10.5194/egusphere-egu26-313, 2026.

EGU26-2630 | ECS | Posters on site | EMRP1.6

Microstructural controls on the quality and fracture toughness of New Zealand nephrite jade (pounamu) 

Natalia Seliutina, Marshall Palmer, Kai Chun Li, David J Prior, Simon C Cox, Nick Mortimer, Anne Ford, and Li-Wei Kuo

Nephrite jade is a monomineralic rock composed of fine-grained interwoven amphibole fibres of the tremolite-actinolite series. This rock has a great cultural importance for many countries due to its combination of beauty, toughness, and high fracture resistance. In New Zealand, nephrite jade (pounamu) is culturally significant to Māori, with a documented history of use in the manufacture of tools, weapons, jewellery, and talismans. Despite this historical importance, there is a lack of systematic quantitative data on the physical and mechanical properties that contribute to its workability and durability.

Traditionally nephrite jade’s suitability for carving has been relying on carvers’ expertise and empirical knowledge. Drawing on the collective experience of Māori artisans, a preliminary survey of pounamu jade carvers (n=20) ranked the quality of a collection of specimens, showing positive correlation between perception of material quality and measured anisotropy in compressional (P-) wave velocity. Current research aims to evaluate the intrinsic origin of this anisotropy and it’s link to mechanical properties through combined microstructural and mechanical analysis.

Electron backscatter diffraction (EBSD) maps of three samples characterised microstructural patterns associated with perceived quality. A sample subjectively rated by carvers as high-quality is noted for homogeneous microstructure with a relatively small grain size (Equivalent diameter on average <8 μm), a weaker crystallographic preferred orientation (CPO) (M-index <0.04), and a lower density of pre-existing microcracks. In contrast, samples identified as poor quality exhibit a stronger CPO (M-indexes 0.14 and 0.09, J-indexes 5.36 and 3.66), particularly within larger grains, greater grain size variability (Equivalent diameter from first μm to 120 μm), and a generally coarser grain size.

Fracture toughness measurements (K1C) were conducted on 3×4×25 mm samples using a universal testing machine equipped with a four-point bending setup, following ISO 6872. Results of these measurements correlate with microstructural observations above. A sample with smaller, more homogeneous grain sizes demonstrates higher fracture toughness. This relationship is consistent with previously described toughening effect related to crack deflection. In nephrite jade, the fracture path is interpreted to be deviated or deflected around the fibres, thereby increasing the effective fracture surface energy. Thus, the coarser microstructures observed in lower-quality samples can contribute to a reduction in this toughening effect, leading to lower fracture resistance. A higher density of pre-existing microcracks observed in coarser-grained samples also leads to lower fracture toughness

Thus, the empirical assessments of nephrite jade quality by carvers correlate with quantifiable microstructural parameters, where a fine-grained, homogeneous fabric with weak CPO promotes crack-deflection toughening and better fracture resistance.

How to cite: Seliutina, N., Palmer, M., Li, K. C., Prior, D. J., Cox, S. C., Mortimer, N., Ford, A., and Kuo, L.-W.: Microstructural controls on the quality and fracture toughness of New Zealand nephrite jade (pounamu), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2630, https://doi.org/10.5194/egusphere-egu26-2630, 2026.

EGU26-5645 | ECS | Posters on site | EMRP1.6

Fault‑Controlled Migration of Geogenic Hydrogen in the Lavanttal Basin (Austria) 

Nils Bezwoda, Martin Schöpfer, Bernhard Grasemann, and Gabor Tari

As society works to reduce carbon emissions and phase out fossil fuels, new and sustainable energy sources are increasingly sought. Hydrogen is typically viewed as an energy carrier, but naturally occurring geogenic hydrogen has emerged as a potential primary energy source. Its appeal, namely zero carbon footprint and continuous generation through subsurface processes, is tempered by major uncertainties. Although the mechanisms that produce natural hydrogen are reasonably well understood, successful exploration cases remain rare and its migration pathways and interactions within the subsurface are poorly constrained.

This project investigates hydrogen migration from a likely ophiolitic source along an active, highly segmented strike‑slip fault system in the Neogene Lavanttal Basin (Austria). We combine short‑term and long‑term soil‑gas measurements with subsurface information from the recently completed Koralm railway tunnel and vintage 2D seismic data. The integrated dataset suggests a possible link between elevated near‑surface hydrogen concentrations and structural features such as subsurface faults and surface lineaments. If confirmed, these results would improve our understanding of hydrogen migration in faulted crust and support more reliable site selection for future natural hydrogen exploration and production.

How to cite: Bezwoda, N., Schöpfer, M., Grasemann, B., and Tari, G.: Fault‑Controlled Migration of Geogenic Hydrogen in the Lavanttal Basin (Austria), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5645, https://doi.org/10.5194/egusphere-egu26-5645, 2026.

EGU26-7492 | Posters on site | EMRP1.6

The formation of hydrogen-emitting “fairy circle” 

Martin Schöpfer, Christine Detournay, and Gabor Tari

Natural hydrogen is emerging as a promising sustainable energy source with a negligible carbon footprint. Among the most striking surface indicators of subsurface hydrogen production are “fairy circles”, distinctive, sub‑circular features marked by anomalous vegetation patterns and subtle topographic depressions, often with depth‑to‑diameter ratios as low as 1:100. While previous numerical studies have examined soil‑gas hydrogen anomalies associated with active fairy circles, the mechanism responsible for the observed surface subsidence has remained unclear.

Here, a geomechanical model grounded in soil‑mechanics principles is developed to explain the formation of these depressions. Using coupled simulations of two‑phase flow and volumetric deformation driven by changes in effective stress, the model reproduces surface expressions consistent with those observed in natural hydrogen‑emitting fairy circles. These results provide a physically plausible mechanism for the development of fairy‑circle topography and offer a framework for interpreting surface indicators of subsurface hydrogen generation.

How to cite: Schöpfer, M., Detournay, C., and Tari, G.: The formation of hydrogen-emitting “fairy circle”, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7492, https://doi.org/10.5194/egusphere-egu26-7492, 2026.

EGU26-9311 | ECS | Posters on site | EMRP1.6

Mechanical control of soft mineralogical phases on the global strength of the rock: the case of anhydrite and gypsum 

Chiara Caselle, Arianna Paschetto, Patrick Baud, Sabrina Bonetto, and Pietro Mosca

The mechanical response of polymineralic rocks is the result of the combination of the individual strengths of all the mineralogical phases that are included in it. But which percentage of a softer mineral is sufficient to soften the mechanical strength of the entire rock? And, on the other hand, which percentage of a stronger material is enough to increase the strength of a soft rock? And do these percentages depend on the microstructure?

Gypsum-anhydrite rocks have the requisites to answer these questions, due to the high mechanical contrast between anhydrite and gypsum mineralogical phases and to the high heterogeneity of microstructures that are usually present even in a single rock mass because of the low temperatures of the phase transition between gypsum and anhydrite.

For these reasons, the present study investigated the strength and creep response under uniaxial compression of Triassic sulphates from the Italian Western Alps. The samples considered may be clustered in three main groups, depending on the occurring microstructural organization of gypsum and anhydrite mineralogical phases: i) pure gypsum, ii) gypsum with relicts of anhydrite at the nuclei of the crystals and iii) anhydrite with gypsum bordering the rims among the crystals.

Results of mechanical tests showed that even a low percentage of anhydrite present at the nuclei of the gypsum crystals strongly controls the mechanical response, causing an increase in the uniaxial strength from 20-25 MPa to 50-70 MPa. On the other hand, the presence of small quantities of gypsum at the rim of anhydrite crystals implies a decrease of mechanical strength of up to 50% with respect to the values expected for pure anhydrite.

Unlike the results about strength, creep strain rate data in gypsum showed a high predictability, suggesting that time-dependent deformation is mainly controlled by mechanisms occurring at the rim of crystals (e.g., pressure solution).

How to cite: Caselle, C., Paschetto, A., Baud, P., Bonetto, S., and Mosca, P.: Mechanical control of soft mineralogical phases on the global strength of the rock: the case of anhydrite and gypsum, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9311, https://doi.org/10.5194/egusphere-egu26-9311, 2026.

EGU26-12392 | ECS | Orals | EMRP1.6

Petrophysical inversion of pore and fracture aspect ratios in complex fractured-vuggy reservoirs using TGCOA algorithm 

Zilong Xiong, Xingyao Yin, Zhengqian Ma, and Wei Xiang

Accurately acquiring elastic and anisotropic parameters is  critical for hydrocarbon prediction. Studies have shown that pore and fracture aspect ratios significantly influence the elastic and anisotropic properties of rocks. However, obtaining accurate pore aspect ratio data is extremely difficult and costly, and conventional logging data typically lack this information. Consequently, pore and fracture aspect ratios are generally assumed to be constant based on experience, which does not accurately reflect the actual geological conditions of the formation. To address this limitation, this study proposes a nonlinear petrophysical inversion method based on the Tetragonula Carbonaria Optimization Algorithm (TGCOA), an algorithm inspired by the nest-building and temperature-regulating behavior of tetragonula carbonaria, notable for its structural simplicity and fast convergence. First, a complex fractured-vuggy petrophysical model and inversion objective function are developed by integrating the Xu-White dual-pore model with the Eshelby-Cheng model. Then, constrained by measured acoustic logging data, the TGCOA global optimization algorithm is employed to perform nonlinear petrophysical inversion, solving for the pore and fracture aspect ratios. Finally, these estimated ratios are used as inputs for the petrophysical model to calculate the elastic and anisotropic parameters of rocks. This method comprehensively utilizes various well-logging data to obtain more accurate elastic and anisotropic parameters. Application of the proposed approach to field data in eastern China demonstrates its high computational efficiency and accuracy.

How to cite: Xiong, Z., Yin, X., Ma, Z., and Xiang, W.: Petrophysical inversion of pore and fracture aspect ratios in complex fractured-vuggy reservoirs using TGCOA algorithm, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12392, https://doi.org/10.5194/egusphere-egu26-12392, 2026.

EGU26-12588 | Posters on site | EMRP1.6

Framework for mersuring deformation of cylindrical sample in 2D DIC  

Antonin Chalé, fengchang bu, michel jaboyedoff, and marc-henri derron

Digital image correlation (DIC) is a powerful tool in lab-scale rock mechanics, yet its application to cylindrical samples is compromised by perspective-induced distortions. These optical effects lead to significant inaccuracies in measuring deformations, especially impacting the reliability of Poisson's ratio calculations. To address this, we developed a specialised preprocessing workflow to rectify raw images before correlation.

The proposed method uses a custom Python script that performs image denoising, camera calibration, and lens distortion correction and an unwrapping algorithm that projects the cylindrical surface onto a 2D plane, effectively "flattening" the sample geometry. This allows standard 2D DIC software, such as NCORR, to process the data without the geometric bias inherent in radial perspectives.

To validate the workflow, results were benchmarked against a 3D-DIC system and physical sensors. Preliminary data shows that our rectification process significantly improves displacement accuracy on lateral surfaces, providing a low-cost yet precise alternative to complex 3D setups. This enhancement is crucial for characterising displacement over the full sample surface where traditional strain gauges are limited. Future work will focus on refining pixel-level interpolation to further minimise noise in high-strain zones.

How to cite: Chalé, A., bu, F., jaboyedoff, M., and derron, M.: Framework for mersuring deformation of cylindrical sample in 2D DIC , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12588, https://doi.org/10.5194/egusphere-egu26-12588, 2026.

EGU26-12906 | ECS | Orals | EMRP1.6

Effect of porosity on anhydrite swelling 

Antonia Nousiou and Erich Pimentel

Swelling in anhydritic claystones remains a major tunnelling risk. Although this phenomenon has been widely studied, knowledge gaps persist regarding its swelling behaviour. One of them being the effect of porosity on the volumetric strains that develop during the anhydrite to gypsum transformation. To address this gap, a series of laboratory tests was carried out on artificial specimens made from highly compacted mixtures of anhydrite and kaolin powders. The initial porosity was varied between 0.22 and 0.35, and volumetric strain development was monitored during gypsum formation. The experiments show that transformation-induced strains decrease with increasing initial porosity. The observations further suggest two distinct mechanisms: in more porous specimens, gypsum precipitation occurs largely within the existing pore space, reducing porosity and limiting bulk expansion; in more highly compacted specimens, gypsum growth forces matrix expansion, leading to larger macroscopic swelling. These results are applicable to porous media where crystallisation may occur within pores. Overall, the experimental campaign provides observations and a dataset that can support the development and calibration of coupled chemo-hydro-mechanical models for anhydrite swelling, enabling more realistic predictions of strain development due to gypsum growth in tunnelling applications.

How to cite: Nousiou, A. and Pimentel, E.: Effect of porosity on anhydrite swelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12906, https://doi.org/10.5194/egusphere-egu26-12906, 2026.

EGU26-13985 | Posters on site | EMRP1.6

Geotechnical Design and Rework in Flysch Excavations: A Case Study from Split, Croatia 

Goran Vlastelica and Daša Salvezani

Flysch rock masses pose significant challenges in geotechnical design due to their pronounced heterogeneity, anisotropy, and susceptibility to disintegration, particularly in deep urban excavations. These characteristics often result in unpredictable slope behavior, requiring a careful combination of geotechnical modelling and practical experience.

This study presents a case of an excavation approximately 11 m high, constructed for a building in the Pujanke area of Split, Croatia, situated in typical Dalmatian flysch. The original design proposed a wide excavation with relatively gentle slopes, based on conservative geotechnical parameters previously validated in similar conditions through the authors’ prior studies. During construction, the designed geometry was not fully respected, and significantly steeper slopes were implemented, leading to localized slope failure. This situation provided a rare opportunity to observe classical disintegration mechanisms, layer interactions, and the influence of flysch heterogeneity on excavation stability, complementing insights from previous research.

Following the collapse, a remediation project was successfully implemented. However, due to subsequent modifications of the excavation geometry and construction conditions, additional design iterations were required on the same slope. These successive redesigns illustrate the core of rework in AEC design, where changes in fundamental assumptions such as geometry, boundary conditions, and construction phasing necessitate repeated reinterpretation of the same geotechnical problem.

A back-analysis of slope stability demonstrated a strong correspondence between previously proposed design parameters and the actual behaviour of the rock mass, confirming their appropriateness and highlighting the critical importance of strict adherence to design assumptions during execution. The study further discusses various technical solutions and their robustness against potential deviations from planned conditions, including minor slope modifications and reinforcement measures.

The results contribute to a better understanding of the behaviour of flysch rock masses in deep excavations and provide practical guidance for safer and more resilient geotechnical design in urban areas with heterogeneous soft rocks, enabling a more stable continuity of design assumptions and a reduction in rework in AEC design.

How to cite: Vlastelica, G. and Salvezani, D.: Geotechnical Design and Rework in Flysch Excavations: A Case Study from Split, Croatia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13985, https://doi.org/10.5194/egusphere-egu26-13985, 2026.

EGU26-14093 | ECS | Orals | EMRP1.6

FDEM numerical calibration of mechanical properties of tuffaceous rocks for slope stability analysis  

Mattia Montagnese, Federico Feliziani, Gian Marco Marmoni, Guglielmo Grechi, Emilie Lemaire, Pooya Hamdi, and Salvatore Martino

The characterisation of tuffaceous soft rocks represents a substantial challenge for slope stability evaluation. The geomechanical behaviour of these materials depends heavily on the microheterogeneity of pyroclastic rocks and varies considerably based on the degree of alteration and water-rock interaction processes.

Tuffaceous lithologies outcrop in a wide variety of areas worldwide, often forming landslide-prone vertical cliffs, both in coastal and continental settings. These instability processes are controlled by progressive rock failure (PRF) mechanisms that govern the enucleation and propagation of fractures, the evolution of which can lead the slope to a state of instability. PRF process can be numerically analysed by adopting hybrid stress-strain numerical solutions able to capture the transition from continuum to discontinuum behaviour. However, these tools require micromechanical input parameters governing the fracture mechanics (e.g., fracture toughness/energy), which are often difficult to calibrate numerically.

This study focuses on the tuffaceous cliffs of Ventotene Island (Italy), highly susceptible to rock-falls and topples and exposed to sea-wave actions, combining laboratory testing and numerical modelling. In the site the mechanisms of progressive fracturing in this type of soft rock and its relationship with environmental forcings are deepened through the design and implementation of the “Ventotene Field Laboratory”. This natural field laboratory, part of EPOS Field-Scale Laboratories, allows the integration of field observation, in situ monitoring data and numerical investigations.

To characterise the mechanical behaviour of the Ventotene tuffs, uniaxial compressive strength (UCS), indirect tensile (Brazilian) and fracture toughness (FT) tests were performed at Aachen Rock Mechanics Laboratory on representative rock samples under both dry and saturated conditions. The laboratory results highlight a strong influence of water content on the mechanical properties of the tuff, with a marked reduction in strength and stiffness under wet conditions. In addition, the thermal properties of the material were also investigated to support thermo-mechanical analyses.

The laboratory test results were used to provide (micro)mechanical input parameters to a FDEM slope numerical model using the Irazu software (Geomechanica Inc.). Overall, the results show that numerical calibration is essential to obtain a tuned parametrisation of tuffaceous soft rocks and to bridge the gap between laboratory-scale measurements and field-scale responses.

The laboratory tests were numerically simulated, and the calibrated parameters have been transferred to a numerical domain representative of the Ventotene sea cliffs. This latter model served to perform accurate slope stability analysis of coastal cliffs, by combining the action of different (marine and environmental) controlling factors.

The calibrated micromechanical parameters also provide a robust basis for future modelling FDEM studies since calibrations of this nature have rarely been conducted on tuffaceous lithologies.

How to cite: Montagnese, M., Feliziani, F., Marmoni, G. M., Grechi, G., Lemaire, E., Hamdi, P., and Martino, S.: FDEM numerical calibration of mechanical properties of tuffaceous rocks for slope stability analysis , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14093, https://doi.org/10.5194/egusphere-egu26-14093, 2026.

EGU26-15924 | Orals | EMRP1.6

Stress evolution within a granular system undergoing subcritical failure: insights from photo-elastic imaging of a 2D glass disc pack 

Seiji Nakagawa, Anne Voigtländer, Yida Zhang, and Benjamin Gilbert

Compacting granular systems composed of brittle materials not only deform but can also fracture. In these systems, stress transmits across grain contacts and forms force chain networks. A fracture can occur when the heterogeneously distributed stress becomes locally high and critical. Here, we use photoelasticity to visualize the evolution of stress distributions within a uniaxially loaded, homogeneous 2D array of discs made of soda-lime glass, a transparent, isotropic non-crystalline material. We run experiments in water-saturated and nominally dry conditions, through loading, holding and unloading periods. We optically and acoustically (via acoustic emissions) monitor the evolution of stress field, bulk deformation, and crack propagation. Photoelasticity data are analyzed by image recognition and processed to map stress distributions. 

Preliminary results show five characteristics that set the fracturing of granular matter apart from continuum solids. First, we can extract the stress transmissions, which, despite the macroscopic homogeneity, show force chains and an inhomogeneous stress field. Second, these stress concentrations lead to a local excess of strength and disc fractures. The birefringence patterns in individual discs are altered by fractures but still carry load. During unloading, the fractures can slip or frictionally lock and the stress acting on them don’t fully relax. Third, unloading and reloading cause cracking before reaching the previous target. Fourth, cracking continues during holding periods in a time-dependent manner; perhaps subcritical crack growth redistributes stresses and thus leads to cascades or spurts of acoustic emission events. Finally, homogeneously highly stressed subdomains of discs develop that confine grains and thus suppress localization and fracturing.

How to cite: Nakagawa, S., Voigtländer, A., Zhang, Y., and Gilbert, B.: Stress evolution within a granular system undergoing subcritical failure: insights from photo-elastic imaging of a 2D glass disc pack, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15924, https://doi.org/10.5194/egusphere-egu26-15924, 2026.

EGU26-17521 | ECS | Orals | EMRP1.6

A digital rock physics workflow for crystalline reservoirs: Developing digital twins through a geologically driven workflow 

Noël-Aimée Keutchafo Kouamo, Martin Balcewicz, Lisa Marie Beiers, Jörg Renner, and Erik H. Saenger

Reliable characterization of crystalline geothermal reservoirs requires linking rock microstructure to effective physical properties across scales, from pore to reservoir level. Digital rock physics (DRP) provides a promising framework by combining three-dimensional imaging with numerical simulation. However, established DRP workflows for sedimentary rocks are often insufficient when applied to crystalline lithologies. Low porosity, complex mineral intergrowths, fine inclusions, and alteration textures complicate phase identification and introduce biases in predicted elastic, permeability, and thermal properties, limiting established DRP workflows for low-porosity crystalline rocks. This study presents a geologically driven workflow for a granitoid rock sample from the Frontier Observatory for Research in Geothermal Energy (FORGE) site in Utah, USA. High-resolution X-ray computed tomography (XRCT) of cylindrical core plugs (10 mm diameter, 40 mm length) at 6.9 µm voxel resolution provides the basis for digital pore-scale analysis. Multiphase segmentation, i.e., assigning gray-scale intensities in XRCT volume to specific mineral phases, was performed by integrating grayscale-based thresholding techniques with geological constraints derived from thin-section petrography and scanning electron microscopy (SEM). This integrated workflow reduces misclassification caused by overlapping gray-scale intensities, partial-volume effects at phase boundaries, and unresolved microporosity. The resulting segmentation distinguishes pore space, quartz, feldspar, ferromagnesian minerals (amphibole, biotite), titanite, and accessory phases (zircon, opaque oxides, apatite). Initial digital twin analysis shows results that deviate from laboratory measurements for porosity and the determined P- and S-wave velocities. We suspect that assigning completely intact single-crystal properties to the segmented phases may be incorrect, as the microstructure provides clear information about mechanical stresses, e.g., undulatory extinction or mineral alignment. Additionally, the analyzed subvolume (4003 with an edge length of 2.76 mm) does not yet constitute a representative volume element (RVE) relative to the coarse feldspar grain size (1-3 mm). This results in the following challenges for a DRP workflow in relation to crystalline rocks compared to established sedimentary rocks: (1) XRCT scans of larger field of views to encounter the larger minerals within the granitoid sample, (2) assigning reduced elastic properties to the individual segmented mineral phases due to microcracks and fluid inclusions, (3) Preserving high-resolution imaging to resolve the small volumes of porosity (~1.2 %). We present a refined DRP workflow that addresses these challenges through multi-scale imaging strategies and microstructure-informed elastic property assignments, validated against laboratory measurements on FORGE crystalline samples.

How to cite: Keutchafo Kouamo, N.-A., Balcewicz, M., Beiers, L. M., Renner, J., and Saenger, E. H.: A digital rock physics workflow for crystalline reservoirs: Developing digital twins through a geologically driven workflow, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17521, https://doi.org/10.5194/egusphere-egu26-17521, 2026.

EGU26-17668 | ECS | Orals | EMRP1.6

Observations of laboratory earthquake rupture: implications for earthquake early warning 

Akos Kiss, Elena Spagnuolo, Chiara Cornelio, Stefano Aretusini, Valeria Longobardi, Massimo Cocco, Jacopo Taddeucci, and Simona Colombelli

The onset of an earthquake is associated with a nucleation phase, which is necessary to create the conditions for the subsequent dynamic rupture propagation. Theoretical models and laboratory experiments have been proposed to compensate for the lack of direct observations of earthquake nucleation, remaining poorly understood and described through conceptual models. A central and unresolved question is whether and how the nucleation and breakout phases influence the subsequent dynamic rupture propagation and arrest and ultimately determine the final earthquake size. Recent seismological evidence points towards weak determinism between nucleation and final earthquake size. 

Here we present the Mechanics of Earthquakes and Extended Ruptures Apparatus (MEERA) - a horizontal multiaxial apparatus designed to nucleate dynamic instabilities on an experimental fault. The extended size of the fault (30 x 5 cm) enables the simulation of rupture propagation under a controlled environment. This provides an opportunity to study physical controls on final rupture size. Surface and along-fault deformation before and during dynamic instabilities are monitored with the help of digital image correlation and fiber optic sensing. In addition, an array of 12 high frequency (10 MHz) acoustic emission sensors record elastic waves radiated from dynamic instabilities. The aim of experiments on MEERA, part of the wider ERC-FORESEEING project, will be to bring observations on natural earthquake data to the scale of laboratory fractures and to understand whether the onset of acoustic emissions signals follows a similar trend with magnitude as observed for small natural earthquakes. We will present preliminary results of experiments showing the emergence of a critical nucleation length for dynamic rupture propagation during experiments and will discuss the implications of these findings for larger scale natural earthquakes, in the context of Earthquake Early Warning applications. 

How to cite: Kiss, A., Spagnuolo, E., Cornelio, C., Aretusini, S., Longobardi, V., Cocco, M., Taddeucci, J., and Colombelli, S.: Observations of laboratory earthquake rupture: implications for earthquake early warning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17668, https://doi.org/10.5194/egusphere-egu26-17668, 2026.

EGU26-18000 | ECS | Orals | EMRP1.6

Assessing Changes in Rock Properties and Tensile Strength due to High Temperature from Laboratory Simulation Studies 

Xuan-Xinh Nguyen, Jan Blahůt, Ondřej Racek, Ghazaal Rastjoo, Artem Polezhaev, and Marco Loche

The effects of high temperature on the tensile strength and physical properties of rocks were investigated using furnace heating and simulated fire treatments. Four rock types—basalt, granite, limestone, and sandstone—were examined under dry, wet, and saturated conditions (0%, 50–60%, and 100% water content, respectively). Tensile strength was measured before and after heating using the Brazilian test, while changes in porosity, thermal conductivity, mass, and P- and S-wave velocities were also evaluated. Thermal measurements indicate that both heating methods reached maximum temperatures of approximately 600 °C and produced comparable effects on rock properties. Initial water content had a negligible influence on post-treatment tensile strength and physical properties. In contrast, rock lithology strongly controlled the degree of thermal damage. Basalt, characterized by high initial tensile strength, exhibited minor reductions in tensile strength and wave velocities, whereas sandstone showed greater degradation. Granite and limestone exhibited pronounced reductions in P- and S-wave velocities. Rocks with higher thermal conductivity, such as sandstone, experienced larger decreases in thermal conductivity after heating, while basalt showed the smallest change. Conversely, basalt exhibited the greatest increases in porosity and mass loss. Overall, rock lithology and initial mechanical strength are the primary factors governing rock degradation under high-temperature exposure.

How to cite: Nguyen, X.-X., Blahůt, J., Racek, O., Rastjoo, G., Polezhaev, A., and Loche, M.: Assessing Changes in Rock Properties and Tensile Strength due to High Temperature from Laboratory Simulation Studies, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18000, https://doi.org/10.5194/egusphere-egu26-18000, 2026.

EGU26-18501 | ECS | Orals | EMRP1.6

When do background fractures form?  

Jasper Hupkes, Pierre-Olivier Bruna, Giovanni Bertotti, Perach Nuriel, Marcel Guillong, and Jérôme Caudroit

Predicting the geometry of natural fracture networks in the subsurface is a challenging endeavor. In this study, we present a model in which burial-related stress curves are combined with the theory of sub-critical crack growth to investigate the timing of propagation of fractures that constitute the background network, i.e. not genetically related to faults and/or folds.

To predict principal stress orientations and magnitudes as a function of crustal depth, we relate the vertical stress to the density of the overburden, and the horizontal stresses are estimated by calculating the Poisson effect caused by this overburden. In addition, we assume a tectonic stress in the direction of the maximum horizontal stress. We correct the resulting values for the effects of pore fluid pressure.

Based on the orientation and magnitude of the principal stresses at various depths, we calculate the normal and shear stresses on planes ideally oriented for opening and shear fractures (perpendicular to σ3 and at 30 degrees with σ1, parallel to σ2 respectively). Following linear elastic fracture mechanics, the normal and shear stresses are used to compute the stress intensity at fracture tips and estimate the related fracture propagation rate adopting sub-critical crack growth theory.

This simplified model gives insight into the relationship between depth and i) magnitudes of horizontal and vertical stresses, ii) permutations of principal stresses and associated changes of stress regimes and iii) the magnitude of fracture stresses driving fracturing.

We test our model in the Lower Cretaceous limestones of the Geneva Basin, a naturally fractured formation targeted for geothermal exploitation. The burial curve of this formation is marked by two distinct burial phases. The first is in the Late Cretaceous with maximum burial depths of +-500 m. After this, the carbonate rocks have been exhumed to the surface in the Paleogene, followed by deep burial (up to 4000 m) in the foreland of the emerging Alpes in the Miocene. Our model predicts that sub-critical fracture growth only occurred during the latest burial phase, in a reverse and strike-slip regime.  

The results are compared with analogue outcrops of the Lower Cretaceous carbonate rocks. Multiple generations of calcite veins from different mountain ranges surrounding the Geneva Basin (Jura, Vuache, Bornes Massif) are sampled for absolute dating with the U/Pb geochronology. The obtained ages confirm a change in stress regime from reverse to strike-slip in the Oligocene to Miocene times

How to cite: Hupkes, J., Bruna, P.-O., Bertotti, G., Nuriel, P., Guillong, M., and Caudroit, J.: When do background fractures form? , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18501, https://doi.org/10.5194/egusphere-egu26-18501, 2026.

EGU26-19502 | ECS | Posters on site | EMRP1.6

Effects of pore fluid chemistry on localised and ductile deformation of porous rocks. 

Francesco Lazari, Gabriel Meyer, Anne Pluymakers, and Marie Violay

In geological reservoirs, pore fluid chemistry significantly impacts rock strength through mineral dissolution, precipitation, and surface charge modifications. Understanding these interactions is crucial for geological applications such as CO₂ storage and geothermal energy applications, where fluid chemistry controls reservoir integrity, exploitability, and aging.

With increasing depth, porous rocks transition from localized to ductile deformation regimes, with the latter characterized by compactant behavior that drastically reduces permeability and affects reservoir exploitability. The role of fluid chemistry in controlling this transition remains poorly understood and varies with fluid composition, mineralogy, and stress conditions.

We performed triaxial deformation experiments on Tavel limestone (84% calcite, 7.5 % quartz and 6% phyllosilicates,14% porosity) at effective confining pressures of 20 MPa (localised regime) and 100 MPa (ductile regime) under constant strain rate (10⁻⁶ s⁻¹). Samples were tested dry and saturated with: deionized water, 0.01 M HCl solution, CO₂-water solution, CaCO₃-saturated solution, 0.1 M MgCl₂, 6 M NaCl and 0.1 M NaOH solutions. During deformation, we continuously monitored spectral electrical conductivity (0.1 Hz–1 MHz), permeability, and P-S wave velocities. Pore fluid chemistry variations were analyzed using ICP-OES, and post-mortem sample were characterized at SEM.

Results reveal water weakening in the localised regime, while in the ductile regime water or fluid chemistry only marginally affect rock strength. These findings contrast sharply with previous results on sandstone under identical conditions (Lazari et al., 2025), where chemical effects were negligible in the localized regime but caused 30-35% weakening during ductile deformation.

In the localized regime, the presence of Mg+2 or CaCO3 leads to a slight increase of peak stress, while the presence of HCl creates dissolution patterns on the sample, though without altering the mechanical properties of the rock in the observed timescale.

Increased pore connectivity is evidenced by increasing electrical conductivity with deformation, while calcite dissolution is testified by increased Ca+2 concentration in the fluid after deformation.

Our results have critical implications for reservoir management: (1) carbonate integrity in shallow reservoirs is more sensitive to formation water chemistry than siliciclastic rocks; (2) CO₂ injection requires careful assessment and evaluation of long-term processes; and (3) rock-specific understanding of chemical-mechanical coupling is essential—behaviors cannot be extrapolated across lithologies. These findings underscore the importance of accounting for specific rock-fluid interactions in geological reservoir management.

How to cite: Lazari, F., Meyer, G., Pluymakers, A., and Violay, M.: Effects of pore fluid chemistry on localised and ductile deformation of porous rocks., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19502, https://doi.org/10.5194/egusphere-egu26-19502, 2026.

Underground storage facilities are receiving increasing interest for a variety of geo-engineering applications in the realm of renewable and sustainable energy: geothermal systems, carbon capture and storage, nuclear waste repository and hydrogen storage. Particularly for the hydrogen storage case, this gaseous fluid in injected and withdrew cyclically, causing variations of the effective stress field of the reservoir and caprock.

Based on the Terzaghi effective stress law, changing the effective stress can be achieved by either changing the principal stress or the pore pressure. The first option, called cyclic loading and unloading, has been used extensively to study the effects of cyclic conditions on the hydro-mechanical properties of different rock types. However, the actual phenomenon occurring in a reservoir rock is the cyclic variation of pore pressure, or cyclic pressurization. The cyclic flow of pressurized fluids may mobilize particles, which can clog fluid pathways, and trigger chemical reactions such as dissolution. This leads to an alteration of the microstructure of the rock matrix differently from that caused by the cyclic loading and unloading case.

Although cyclic pressurization experiments cannot be run on every rock at the laboratory scale due to poor hydraulic properties, we chose a highly porous and permeable rock, Bentheim sandstone, which guarantee us a pore pressure equilibrium throughout a rock sample during this type of experiment. Apart from its hydraulic properties, Bentheim sandstone is regarded as a conventional georeservoir rock even at great depth, due to its mineral composition, homogeneity, micro- and macrostructure. Therefore, it has been extensively tested for a variety of applications to understand its physical and mechanical properties under changing environmental conditions.

As part of the TEN.efzn project, we performed a series of laboratory experiments on both intact and fractured rock samples, carried out in a servo-controlled triaxial apparatus, capable of simulating in-situ pressure and temperature conditions at relevant depths. By combining mechanical and hydraulic data with acoustic emission and ultrasonic velocity data, we observe that cyclic pressurization leads to higher sample compaction compared to cyclic loading and that the presence of a fracture zone leads to higher changes of the hydro-mechanical properties.

Our results suggest that the values of specific properties obtained during cyclic loading experiments underestimate the real values of reservoir rocks under cyclic fluid injection and withdrawal.

How to cite: Fazio, M., Gottlieb, M., and Sauter, M.: Experimental study on the variation of hydro-mechanical properties of reservoir rocks under cyclic loading and cyclic pressurization  , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19936, https://doi.org/10.5194/egusphere-egu26-19936, 2026.

EGU26-21233 | Posters on site | EMRP1.6

The influence of porosity and microstructure on the fracture toughness of basalts from Mt. Etna: laboratory measurements 

Leonie Papanagnou, Séverine Furst, Corentin Noël, Michael J. Heap, Marie Violay, and Morelia Urlaub

Mode I fracture toughness, KIc, is a key measure of rock strength. In volcanology, KIcis particularly relevant for dike propagation, as it quantifies the critical stress intensity factor required for fracture propagation under tensile stress. KIc has been extensively studied for rock types and construction materials relevant to civil engineering, mining, and hydrocarbon-related applications. However, there is a paucity of data for volcanic rock. In this study, we present KIcvalues for basalt samples of varying porosity and texture from four different lava flows on Mt. Etna (Italy) and investigate the influence of key microstructural parameters on KIc.

We conducted 12 mode I fracture toughness experiments under dry, ambient pressure conditions on Cracked Chevron-notched Brazilian Disc specimens and determined KIc using a standardised method. Additionally, we characterised rock physical properties including porosity, elastic wave velocities, and permeability, and analysed thin sections to determine mineralogical composition and rock texture. We compared the physical and microstructural properties of the four lavas and then assessed those properties regarding any correlations with KIc.

The fracture toughnessmeasurements were successful for 10 of the 12 specimens, yielding KIcvalues of 0.61.3 MPa·m1/2. Average connected porosity varied between 9­ and 17%. P-wave velocities varied from 3.1 to 3.8 km/s, while permeability varied from 6.7·10-17 to 6.3·10-12 m2.

Our fracture toughness data are consistent with experimental data from the literature, fitting the general trend of high KIc typically corresponding to low porosity. However, within our small data set of rather heterogenous porosity characteristics and rock textures, we observe no strict inverse correlation of KIc,and porosity, since the porosity range of our samples is only moderate and other microstructural factors (e.g. pore size and shape) can dominate fracture behaviour in individual cases. We observe no systematic relationship between elastic wave velocities and KIc.

How to cite: Papanagnou, L., Furst, S., Noël, C., Heap, M. J., Violay, M., and Urlaub, M.: The influence of porosity and microstructure on the fracture toughness of basalts from Mt. Etna: laboratory measurements, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21233, https://doi.org/10.5194/egusphere-egu26-21233, 2026.

EGU26-21311 | Posters on site | EMRP1.6

From grain-scale dissolution to reactive fracture: A multiscale geomechanical study of chemo-mechanical couplings in reservoir rocks 

Hadrien Rattez, Alexandre Sac-Morane, Fanyu Wu, Manman Hu, and Manolis Veveakis

Chemical weathering induced by reactive fluid circulation critically affects the mechanical properties of sedimentary rocks involved in subsurface energy applications such as geothermal systems and underground energy storage. This work investigates chemo-mechanical degradation in bonded granular geomaterials through a multiscale approach combining discrete and continuum modeling.

At the grain scale, Discrete Element Method (DEM) simulations are used to study dissolution-driven debonding under oedometric conditions. The evolution of the lateral earth pressure coefficient k0 used as a proxy for stress state, is analyzed as a function of cementation degree, confining pressure, initial stress anisotropy, and loading history. Progressive dissolution leads to convergence toward an attractor stress state, with k0 stabilizing between 0.3 and 0.4 independently of initial conditions. This behavior results from the collapse of cement-stabilized force chains and chemical softening of grains.

At the continuum scale, a phase-field fracture model coupled with damage-enhanced reactive diffusion is developed, informed by micromechanically derived degradation laws from DEM simulations. The model reveals that higher initial cementation delays brittle fracture initiation, while increased acidity may induce a chemical ductilization effect that counter-intuitively postpones fracture due to localized softening ahead of crack tips. The competing effects of chemical softening and degradation of fracture toughness are quantitatively characterized.

How to cite: Rattez, H., Sac-Morane, A., Wu, F., Hu, M., and Veveakis, M.: From grain-scale dissolution to reactive fracture: A multiscale geomechanical study of chemo-mechanical couplings in reservoir rocks, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21311, https://doi.org/10.5194/egusphere-egu26-21311, 2026.

EGU26-21876 | ECS | Orals | EMRP1.6

Experimental and numerical study of a landslide in a complex geostructural context: the case of Calita (Italy) 

Alessandro Fraccica, Mauro Bonasera, Danilo D'Angiò, Gianluigi Di Paola, Matteo Maggi, Vittorio Chiessi, Gennaro Maria Monti, Federica Pellegrini, Nicola De Simone, and Roberto Spagni

The Calita landslide (Northern Apennines, Italy) is a large, complex phenomenon extending over approximately 0.9 km² and characterized by a roto-translational rockslide, in a flysch-dominated area, that evolves downslope into an earth slide–earthflow covering a length of approximately 2.5 km. The earthflow sector involves clay-rich soils derived from a chaotic and strongly tectonized melange partially mixed with the progressively degradated rocky head scarp. Landslides of this type are highly sensitive to hydro-mechanical perturbations, including pore water pressure increases and undrained–drained mechanisms induced by static loading. Moreover, the litho-structural setting controls deep filtration pathways, potentially promoting localized pressurization beneath the sliding surface.

This contribution presents ongoing work aimed at developing a geotechnical model of the Calita landslide and identifying its predisposing and triggering factors. Geological surveys, field instrumentation, laboratory tests have been integrated to characterize the hydro-mechanical behaviour of the landslide body. Direct shear, oedometer, triaxial and water retention tests were performed, allowing derivation of strength parameters, permeability, and pore pressure response under saturated and partially saturated conditions. Mineralogical analyses revealed the presence of gypsum and pyrite along the landslide’s shear surfaces, indicating possible chemo-mechanical weakening mechanisms and enhanced fluid–rock interaction.

GNSS, inclinometer, and piezometric monitoring delineated the spatial variability of displacement and hydraulic pressures, with piezometers recording artesian conditions in some portions of the earth slide-earthflow. DEM of differences were produced on high-resolution Digital Terrain Models obtained during the monitoring years, from 1973 to 2024, allowing to appreciate the areas where displacements occurred and the related mobilized volumes. Finally, numerical analyses were carried out using both finite element (hydro-mechanical) and limit equilibrium approaches to evaluate slope stability under different hydraulic regimes. The results provide a consistent geotechnical framework for future scenario analyses and mitigation planning.

How to cite: Fraccica, A., Bonasera, M., D'Angiò, D., Di Paola, G., Maggi, M., Chiessi, V., Monti, G. M., Pellegrini, F., De Simone, N., and Spagni, R.: Experimental and numerical study of a landslide in a complex geostructural context: the case of Calita (Italy), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21876, https://doi.org/10.5194/egusphere-egu26-21876, 2026.

The total organic carbon content is one of the key controls on hydrocarbon potential in unconventional shale systems. In the Indian Barren Measures Shales, TOC estimation from wireline logs remains challenging due to the strong heterogeneity, variable mineralogy, and limited core-calibrated geochemical measurements of shales. Standard empirical methods, such as the ΔlogR technique, capture first-order trends but often fail to generalise across mineral compositions. Purely data-driven machine learning models improve flexibility but may produce physically inconsistent predictions when sample sizes are small or when petrophysical responses are nonlinear.

This work presents a Physics Informed Convolutional Neural Network designed to estimate TOC from gamma ray, bulk density, and resistivity logs while embedding rock physics behaviour directly into the learning process. The network uses one dimensional convolutional filters to learn depth dependent patterns associated with organic richness, and incorporates the ΔlogR principle as a soft constraint in the loss function. The training workflow includes depth windowing and a hybrid loss function that balances data fidelity with physics consistency, which stabilises learning under limited sample availability.

Using 104 depth-indexed TOC measurements, the model was trained with five-fold cross-validation and a range of physics weighting factors. The final configuration achieved a mean absolute error (MAE) of 0.3, a root mean square error (RMSE) of 0.4, and a Pearson correlation coefficient (r) of 0.9, representing an improvement over both a standard multilayer perceptron (MAE = 0.6, RMSE =1, r =0.6) and the classical ΔlogR approach (MAE = 0.9, RMSE =1.3, r =0.4). These results show that physics informed learning provides a reliable and physically consistent framework for petrophysical characterisation in heterogeneous unconventional reservoirs, offering a generalizable workflow that integrates geological knowledge with machine intelligence to support improved formation evaluation and reduce uncertainty in reservoir assessment.

How to cite: Shaik, N. A. and Vedanti, N.: Physics informed convolutional neural network for TOC estimation in heterogeneous Barren Measures Shales, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-232, https://doi.org/10.5194/egusphere-egu26-232, 2026.

The precise quantification of mineral composition is a basis for the accurate geomechanical evaluation, brittleness assessment, and completion design of shale reservoirs. Currently, elemental logging has become an indispensable technical method for acquiring key mineral composition information. The standard industry practice involves solving an optimization problem to invert elemental dry weight fractions, measured downhole, into mineral contents. The accuracy of this inversion is fundamentally governed by a predetermined transformation matrix, which ideally requires rigorous calibration against a statistically robust suite of laboratory X-ray diffraction (XRD) analyses from rock samples. This prerequisite poses a significant constraint in poorly cored intervals, leading to substantial uncertainties in the derived mineralogy.

To reduce the core-dependency, the key innovation lies in formulating the element-to-mineral transformation as a joint inversion problem. The proposed algorithm operates by treating the transformation matrix not as a fixed input but as an optimizable variable within the inversion framework. Starting from a geologically reasonable initial model based on regional knowledge, the method employs an iterative optimization loop. In each cycle, it simultaneously adjusts the mineral volumes and refines the transformation matrix to minimize a dual-objective function. The misfit between the log-measured and model-predicted elemental yields, and a regularization term that constrains the matrix adjustments to physically plausible ranges. The iteration converges when the global error is minimized, yielding a formation-specific optimal transformation matrix alongside the final mineralogy.

The efficacy of the method was rigorously tested using data from offshore shale oil wells in China. Comparative analysis demonstrates that the mineralogical profiles produced by the iterative method achieve an excellent correlation with those derived from the XRD-calibrated approach in intervals where core data is available. More importantly, in zones lacking core control, the iterative method provides stable and geochemically consistent results. A detailed comparative analysis indicates that this method significantly enhances the prediction accuracy for critical brittle minerals such as quartz and plagioclase. The reduction in error for these key components directly translates to higher confidence in computed geomechanical properties.

In conclusion, this study presents a robust workflow that significantly enhances the reliability of mineralogical evaluation from elemental logs in core-constrained environments. The iterative inversion method reduces the critical need for extensive, expensive core-based calibration, offering a powerful and practical tool for the accurate and efficient characterization of offshore shale oil reservoirs. This advancement holds substantial value for optimizing drilling, completion, and stimulation strategies, thereby supporting the economical development of complex unconventional resources.

How to cite: Wang, M., Yin, L., and Yan, W.: An Iterative Inversion Method for Mineral Composition Evaluation in Offshore Shale Reservoirs Based on Elemental Logging, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1443, https://doi.org/10.5194/egusphere-egu26-1443, 2026.

Shale reservoirs, characterized by intricate fluid occurrence,elevated clay and organic matter (OM) contents, and diverse pore structures, present complexities that obscure the primary controlling factors of lacustrine shale conductivity and render existing saturation models insufficient in accuracy. Taking the medium-high maturity lacustrine shale of the Qing1 Member in the Changling Sag, Southern Songliao Basin as an example,  we use 2D nuclear magnetic resonance and pressure-maintained and sealed coring techniques to obtain the original fluid information of shale reservoirs. By combining geochemical, mineralogical, and geophysical properties, we investigate the impact of mineral components, physical properties, and fluid occurrence on the electrical conductivity properties of shale reservoirs. The clay and carbonate minerals play a primary role in  influencing the conductivity of shale, whereas effective porosity plays a secondary role. Conductivity variations within single lithologies are affected by total organic carbon and fluid types. A novel resistivity-saturation interpretation model, which is a function of saturation, for mature lacustrine shale (MLS) is developed based on lithologic distinctions and the influence of OM. This model identifies two primary conductive pathways: free water conduction in matrix pores and additional conduction from clay-bound water. The bound water cementation indexmwb and conductive bound water fraction Swb are introducedto reflect the impact of OM on clay additional conductivity. Compared with the Archie model developed for clay-free rockand the Indonesian model used for shales, the MLS model offers a more accurate calculation of oil saturation in MLS. Our approach makes a step ahead toward reducing uncertainty in  the evaluation of MLSs as potentially economic oil reservoirs. 

How to cite: Li, Z.: Conducting mechanism and saturation model of mature lacustrine shales: A case study of the first member of the Qingshankou Formation in the Changling Sag, Southern Songliao Basin , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1767, https://doi.org/10.5194/egusphere-egu26-1767, 2026.

EGU26-1966 | ECS | Orals | EMRP1.9

LGAF‑FracNet: A Dual‑Backbone Deep Learning Framework for Intelligent Fracture Identification in Electrical Imaging Logging 

Huazhong Yang, Chong Zhang, WenHao Xiong, and JiaHui Zhang

Electrical imaging logging provides rich information on reservoir petrophysical properties and geological features. Fracture identification based on image logs is of great significance for accurate production prediction and reliable estimation of hydrocarbon reserves. However, in electrical imaging log images, fractures typically appear as elongated, low-contrast targets with strong sensitivity to structural continuity. Moreover, variations in formation conditions, imaging parameters, and noise characteristics across different wells pose substantial challenges to existing fracture identification methods, particularly in terms of fine-scale fracture continuity recognition and cross-well generalization. To address these challenges, this study proposes a dual-backbone deep learning framework, termed LGAF-FracNet, for fracture identification in electrical imaging logs. The proposed framework parallelly integrates a convolutional neural network and a Transformer architecture to model local texture features and global semantic relationships, respectively. Considering the circumferential structural characteristics of electrical imaging logs, a liquid ordinary differential equation–based dynamic feature evolution module, an adaptive graph fusion module, and a stripe-aware pooling strategy are incorporated to enhance the representation of elongated and subtle fracture geometries. In addition, a multi-decoder consistency supervision mechanism is introduced to improve cross-well generalization performance. The proposed method is evaluated on a dataset comprising approximately 3,000 electrical imaging log images collected from 21 wells in the Sichuan Basin, covering conductive fractures, resistive fractures, drilling-induced fractures, and bedding structures. A standardized dataset is constructed through manual annotation and data augmentation. Experimental results demonstrate that LGAF-FracNet consistently outperforms mainstream segmentation models in terms of mIoU, F1-score, and pixel accuracy, exhibiting significant advantages in fine-scale fracture continuity, morphological consistency, and cross-well adaptability. These results indicate that the proposed method provides a reliable technical solution for intelligent fracture identification and quantitative characterization in electrical imaging logging.

How to cite: Yang, H., Zhang, C., Xiong, W., and Zhang, J.: LGAF‑FracNet: A Dual‑Backbone Deep Learning Framework for Intelligent Fracture Identification in Electrical Imaging Logging, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1966, https://doi.org/10.5194/egusphere-egu26-1966, 2026.

The effective stress coefficient (ESC) is an important parameter in formation pressure prediction and formation stress estimation, which is usually obtained by experiments and by the empirical function formulas of ESC and porosity. However, the calculation accuracy of these empirical formulas is often affected by lithology and critical porosity, and their application in the whole area or multi-lithology formations is limited. In addition, shear wave velocity data is limited by cost and technical conditions in practical logging applications. Therefore, based on the Gassmann equation and the approximation of P-wave modulus and volume modulus, this study realizes a multi-lithology ESC estimation method using P-wave velocity, density, and porosity, and applies it to the logging of the study block. The dynamic ESC along the wellbore direction is obtained, and the logging dynamic ESC estimation model is corrected to verify the reliability of the method. The results show that the logging-derived ESC is mainly distributed in the range of 0.3~0.8, while the average ESC measured in the laboratory is between 0.5~0.6. The ESC of the sandstone layers with high porosity is relatively large, and that of the mudstone layers with low porosity is small. In the absence of shear wave velocity, this method can effectively estimate the ESC and further predict formation pressure, which plays an important role in oil exploration and development.

How to cite: Wang, X.: Research on the Calculation Method of Dynamic Effective Stress Coefficient Based on P-Wave Velocity, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2114, https://doi.org/10.5194/egusphere-egu26-2114, 2026.

EGU26-2181 | Orals | EMRP1.9

Metalliferous Brine Exploration and Reservoir Intelligent Identification in Qaidam Basin, Northwestern China 

Cheng Chen, Hao Zhang, Xinxin Fang, Yuanjian Zhou, and Yuwei Xia

Metalliferous brine represents a globally significant strategic mineral resource. The western Qaidam Basin in Qinghai, China, harbours immense potential for deep metalliferous brine deposits, yet exploration remains limited due to technical challenges such as the difficulty in identifying deep brine-bearing reservoirs and inaccuracies in delineating their spatial distribution. This paper focuses on the core technological methodology of integrated well and seismic data for deep metalliferous brine detection and intelligent reservoir identification. It comprehensively utilises geological, seismic, and logging data from oil and gas exploration in the western Qaidam Basin to conduct research on multi-source geophysical data fusion and intelligent interpretation. A systematic analysis of brine layer response characteristics in logging (e.g., low resistivity, low natural gamma) and seismic data was conducted. For the first time, seismic forward modelling clearly defined the identification resolution limits of onshore seismic data for halite-bearing sand bodies at primary frequencies of 25–50 Hz: Effective identification requires sandbody interlayers ≥1 metre and single sandbody thickness ≥7–8 metres. Overlapping sandbodies with elevation differences <6 metres are prone to misinterpretation as single layers, while low-velocity interlayers may cause strong reflections to drown out brine-bearing layer signals. This provides crucial theoretical support for practical data interpretation. Building upon this, an innovative approach combining well-logging and seismic data inversion with intelligent recognition based on a deep neural network (UNet++) was proposed. By integrating the high resolution of logging with the lateral continuity advantage of seismic data, automated and high-precision identification of brine layers was achieved. The research successfully established a brine-bearing layer prediction model, enabling quantitative forecasting of the spatial distribution of metalliferous brine layers in the western Qaidam area. This provides scientific justification for subsequent drilling deployment in target zones. It significantly enhances the exploration efficiency and intelligence level for deep metalliferous brine, holding substantial scientific significance and practical value for advancing mineral resource reserves and production.

How to cite: Chen, C., Zhang, H., Fang, X., Zhou, Y., and Xia, Y.: Metalliferous Brine Exploration and Reservoir Intelligent Identification in Qaidam Basin, Northwestern China, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2181, https://doi.org/10.5194/egusphere-egu26-2181, 2026.

EGU26-2499 | Orals | EMRP1.9 | Highlight

Mechanical and Acoustic Dynamic Evolution of Shale under Water-Shale Interaction 

Jian Xiong, Han Fang, Xiangjun Liu, Lixi Liang, and Yi Ding

Water-based drilling fluid invasion-induced shale hydration is one of the key mechanisms leading to shale formation instability. Its essence lies in the microstructural damage caused by hydration, which further leads to the deterioration of mechanical and acoustic properties. To thoroughly investigate the intrinsic relationship of the evolutionary characteristics of “hydration–structural damage–mechanical weakening,” shale samples from the Da’anzhai Formation in the Sichuan Basin were selected. A series of comprehensive experiments were designed, covering different fluid systems, immersion pressures , and immersion times. By conducting simultaneous acoustic (velocity and attenuation), rock mechanical (triaxial), and CT scanning tests, the evolution trends of macro- and microstructures, mechanical properties, and acoustic characteristics of shale under water–rock interaction were quantitatively characterized. The response relationship between mechanical and acoustic parameters was clarified, and the influence of different drilling fluid systems on formation collapse pressure was compared, providing a quantitative basis for drilling fluid optimization. The main conclusions are as follows:
(1) Macro- and microstructural damage exhibits time- and pressure-dependent behavior. After immersion in drilling fluid, macroscopic fractures appeared on the shale surface. CT scanning indicated that hydration-induced fractures primarily formed during the initial immersion stage. With prolonged immersion time or increased pressure, existing fractures continued to expand, while the number of new fractures gradually decreased, reflecting irreversible cumulative hydration damage within the shale.
(2) Mechanical and acoustic parameters exhibit a synergistic deterioration trend. As immersion time and pressure increase, shale acoustic wave velocity, peak amplitude, compressive strength, and elastic modulus all decrease, while the acoustic attenuation coefficient increases. Microscopically, this is attributed to hydration-induced microcrack propagation and mineral interface weakening, which complicate wave propagation paths and intensify energy dissipation, leading to a simultaneous reduction in mechanical performance.
(3) Drilling fluid modification effectively inhibits hydration damage. Compared with the original water-based drilling fluid, adding 3% plugging agent increased shale longitudinal wave velocity and compressive strength by 8.2% and 10.2%, respectively. Using 50% organic salt as an inhibitor increased these values by 12.4% and 22.3%, respectively. When both were used in combination, the improvements further increased to 14.7% and 27.2%. This indicates that physical plugging and chemical inhibition can significantly mitigate structural damage and mechanical weakening.
(4) The acoustic attenuation coefficient is a sensitive indicator for evaluating structural damage. After water–rock interaction, the correlation between shale compressive strength, elastic modulus, and acoustic wave velocity is weaker, while the correlation with the acoustic attenuation coefficient is stronger. This suggests that the acoustic attenuation coefficient responds more sensitively to microstructural damage and can serve as a non-destructive evaluation method for optimizing drilling fluid systems.
(5) Drilling fluid optimization significantly reduces collapse pressure risk. As immersion time or pressure increases, the incremental collapse pressure of the shale formation gradually rises, reaching 0.248 g/cm³ and 0.201 g/cm³ under conditions of 15 days and 7 MPa, respectively. After adding 3% plugging agent, 50% organic salt, and their combination, the incremental collapse pressure decreased to 0.167, 0.151, and 0.113 g/cm³, respectively. This confirms that optimizing drilling fluids through physical–chemical synergy can effectively enhance wellbore stability.

How to cite: Xiong, J., Fang, H., Liu, X., Liang, L., and Ding, Y.: Mechanical and Acoustic Dynamic Evolution of Shale under Water-Shale Interaction, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2499, https://doi.org/10.5194/egusphere-egu26-2499, 2026.

EGU26-2531 | ECS | Posters on site | EMRP1.9

A multiple review on identification and fine evaluation of shale pores: Prospects and challenges 

Qiyang Gou, Shang Xu, Qianzhu Xiong, and Zhen Li

Accurate evaluation of pore systems in shale reservoirs is critical for understanding fluid flow, gas storage capacity, and overall reservoir performance. Extensive research has been conducted on the micro- and nano-pore structure of shale reservoirs using various experimental methods and shale samples. However, discrepancies in sample preparation standards and experimental parameters—such as observation techniques and data interpretation—raise concerns about the reliability and comparability of these results across different shale reservoirs. This review systematically evaluates the current methods for characterizing shale pore systems, with particular emphasis on commonly used techniques such as scanning electron microscopy (SEM), gas adsorption, and CT scanning. Key challenges related to sample preparation (e.g., sample size) and experimental conditions (e.g., voltage and current) are discussed, as these factors can introduce significant inaccuracies into pore structure characterization, even for well-established methods. Additionally, we examine the difficulties in integrating these methods to achieve a comprehensive understanding of shale pore parameters, including the quantification of organic and inorganic porosity, full-scale pore size distribution, and pore connectivity. Addressing these challenges requires the establishment of standardized processing workflows to enhance the comparability of results and minimize experimental errors. We also highlight often-overlooked issues, such as the potential discrepancy between pore structures observed under laboratory conditions and those at in-situ depths. The review concludes with recommendations for future research, including the development of advanced experimental techniques and more efficient data processing strategies to improve pore characterization in shale reservoirs. This review provides a new perspective for future research and addresses a critical gap in understanding the impact of experimental conditions on pore structure characterization outcomes.

How to cite: Gou, Q., Xu, S., Xiong, Q., and Li, Z.: A multiple review on identification and fine evaluation of shale pores: Prospects and challenges, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2531, https://doi.org/10.5194/egusphere-egu26-2531, 2026.

The Ordos Basin is a core area for deep coalbed methane (CBM) accumulation and production in China. The No. 8 coal seam at the Benxi Formation top is a primary target due to its wide distribution, stable thickness, and good gas-bearing capacity. However, complex roof/floor lithology and coal heterogeneity lead to intricate petrophysical responses of mechanical parameters, affecting fracturing efficiency. Thus, an integrated system incorporating rock properties for mechanical parameter prediction, in-situ stress calculation, and fracturability classification is critical for deep CBM sweet spot identification.

Sixty core samples of major lithologies (limestone, mudstone, sandstone, coal rock) were collected from the central-eastern Ordos Basin. Comprehensive laboratory tests were performed, including X-ray diffraction (XRD), uniaxial/triaxial compression, Brazilian splitting, and basic physical tests (P-/S-wave velocity, density). For coal rock, an extended Gassmann-based petrophysical model was established via Biot’s porous medium theory, incorporating pore-fracture extrusion-spray flow effect to accurately predict cleat density. Pearson correlation analysis identified key factors governing mechanical parameters: acoustic velocity, density, cleat density for coal; acoustic velocity, density, shale content for roof/floor rocks. Multiple nonlinear regression models were built for their mechanical parameters, with R²>0.75 between predicted and measured values, ensuring high accuracy.

Using the predicted rock mechanical parameters, the combined spring model was employed to calculate the in-situ stress of the coal-bearing strata. The prediction results demonstrated excellent consistency with field measured data, with an average relative error of less than 10%. Focusing on CBM reservoirs, relevant parameters were extracted, including rock mechanical properties (USC, E, V……) and in-situ stress components (σH, σh……). The correlation between these parameters and single-well daily gas production was systematically analyzed. The XGBoost ensemble learning algorithm was utilized to screen key influencing parameters from high-dimensional data, identifying four critical factors: minimum horizontal stress difference between reservoir and roof, reservoir horizontal stress difference, reservoir tensile strength, and reservoir elastic modulus. A fracturability evaluation model (FI) was constructed based on these key factors, and clustering analysis was applied to classify reservoir fracturability through iterative updating of cluster centers. The classification results yielded three reservoir grades: Class Ⅰ (FI > 0.32) with excellent fracturability, facilitating the formation of complex fracture networks; Class Ⅱ (0.21 < FI ≤ 0.32) with moderate fracturability, tending to form relatively simple fracture networks; and Class Ⅲ (FI ≤ 0.21) with poor fracturability, for which fracturing stimulation is not recommended.

The results of this study show great potential in evaluating deep CBM in the basin. It significantly improves the accuracy of parameter prediction (R² > 0.75) and in-situ stress calculation (error < 10%). Meanwhile, the combination of the FI model and classification standard effectively enhances evaluation precision and decision-making efficiency, providing strong support for targeted fracturing and sustainable deep CBM development.

How to cite: Luo, J. and Xiong, J.: Prediction of Rock Mechanical Parameters in Deep Coal-Bearing Strata and Fracturability Classification Evaluation of Coalbed Methane Reservoirs, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2550, https://doi.org/10.5194/egusphere-egu26-2550, 2026.

EGU26-2639 | ECS | Posters on site | EMRP1.9

Sedimentology Dominated Accumulation Mechanism of Marine Shale Gas 

Xianglin Chen

Recent shale gas drilling wells in southern China confirms significant resource potential within the Lower Carboniferous marine shale of the Yaziluo Rift Trough, yet exploration efficiency is hindered by poorly understood sedimentological heterogeneity and gas accumulation mechanisms. This study integrates major and trace elements, high-resolution field emission scanning electron microscopy, and adsorption analyses (low-pressure N₂/CO₂, high-pressure CH₄) to systematically characterize sedimentary facies, reservoir properties, and gas enrichment patterns. The trough exhibits an asymmetric "platform-basin" model with three distinct sedimentary facies. Basin facies comprise siliceous shale formed in deep-water anoxic settings, yielding the highest total organic carbon (TOC) content (average 3.63%) controlled by redox conditions and paleoproductivity. Lower slope facies consist of mixed shale in dysoxic environments, with moderate TOC (average 1.80%), dominated by redox conditions. Upper slope facies are calcareous shale in shallow, weakly reducing settings, showing the lowest TOC (average 0.99%), influenced by clay-mediated organic preservation. Reservoir analysis reveals that basin facies are dominated by organic pore, whereas lower slope facies display reduced organic pores but increased inorganic pores and micro-fractures, and upper slope facies shift predominantly to inorganic pores and microfractures. Moving from basinward to upper slope, increasing carbonate content expands dissolution pore networks, yet declining TOC diminishes organic pore development, promoting organic-clay complexes and weakening pore structure. Additionally, three shale associations classified by shale-to-argillaceous limestone ratios correspond to specific sedimentary facies. The lower slope shale association demonstrates optimal gas preservation due to high TOC, argillaceous limestone interlayers acting as direct caps, and fracture-enhanced porosity facilitating gas migration. The upper slope association shows promise for self-sealing bodies via acid fracturing despite lower TOC. In contrast, the basin facies shale association exhibits constrained gas retention capacity owing to clay-dominated mineralogy and absence of argillaceous limestone interlayers. This study emphasizes the critical role of lithofacies heterogeneity and integrated "source-reservoir-seal" configurations in evaluating of shale gas accumulation under "slope-basin" depositional architectures, providing a theoretical basis for reservoir development in analogous geological settings.

How to cite: Chen, X.: Sedimentology Dominated Accumulation Mechanism of Marine Shale Gas, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2639, https://doi.org/10.5194/egusphere-egu26-2639, 2026.

Abstract: Buried hill reservoirs in the eastern South China Sea exhibit highly heterogeneous mechanical properties and complex fracture networks that exert significant control on reservoir productivity, fluid pathways, and wellbore stability. Their tectonic evolution, multistage deformation, and lithological diversity make traditional fracture prediction methods insufficient for supporting safe and efficient offshore drilling operations. To address these challenges, this study develops a new integrated framework that combines geomechanical analysis, finite-element numerical simulation, and multi-source geological and geophysical data to characterize fracture attributes and predict fracture behavior under present-day stress conditions. The workflow incorporates acoustic and imaging logging data, high-resolution seismic attributes, lithology-based mechanical property modeling, and 3D Mohr circle stress analysis. These datasets are used to construct a heterogeneous geomechanical model that captures the spatial variability of elastic and strength parameters across the buried hill. Numerical simulations are performed to evaluate the distribution of stress perturbations associated with structural relief and lithological layering, and to assess the likelihood of fracture initiation, propagation, and reactivation under different stress regimes. The results demonstrate pronounced variations in fracture intensity and failure potential both laterally and vertically. Zones near faulted structural highs exhibit locally elevated differential stress and shear strain concentration, leading to enhanced fracture connectivity and increased reactivation probability. In contrast, massive crystalline units and mechanically strong lithologies show limited deformation and lower fracture susceptibility. By integrating the simulated stress field with observed fracture indicators, the study identifies high-risk intervals with elevated risks of borehole collapse, drilling fluid loss, or induced fracturing, as well as fracture-favorable sweet spots that may enhance reservoir penetration and productivity. Furthermore, the framework provides quantitative guidance for optimizing well trajectories, selecting safe drilling windows, and improving well placement strategies in offshore buried hill settings. The results highlight the importance of incorporating geomechanical constraints into fracture characterization workflows to reduce drilling uncertainty and improve the reliability of fracture prediction models. This integrated analytical–numerical approach offers a robust and transferable methodology for evaluating fracture development in complex tectonic reservoirs. It provides practical insights into wellbore stability management, reservoir development optimization, and risk mitigation in the challenging geological environment of the eastern South China Sea. The proposed workflow can also be adapted to similar buried hill or basement reservoirs worldwide.

Keywords: fracture characterization; geomechanical modeling; finite-element simulation; buried hill reservoirs; in-situ stress analysis; south China Sea

How to cite: Deng, C., Tan, J., and Yin, L.: An integrated geomechanical–numerical simulation framework for fracture characterization and prediction in buried hills of the eastern south China Sea, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2650, https://doi.org/10.5194/egusphere-egu26-2650, 2026.

     In deep coal seams, the primary storage space for adsorbed methane resides in the micropores and associated adsorption surfaces of the coal matrix, whereas the fracture network provides the dominant pathway for gas–water transport. Fractures promote the migration and local enrichment of free gas, with their connectivity exerting a fundamental control on methane desorption efficiency and overall seepage capacity. Therefore, elucidating the pore‑scale mechanisms of gas‑driven water displacement is critical for understanding gas–water occurrence and flow dynamics, as well as for assessing the reservoir‑controlling role of different microstructures.In light of the pronounced heterogeneity of coal, this study constructs two pore‑scale digital core models—a matrix‑pore model and a pore–fracture model—based on micro‑CT imaging of low‑rank coal. Utilizing the Volume of Fluid (VOF) method within an immiscible two‑phase displacement framework, we simulate methane‑driven water displacement under reservoir‑formation conditions. The simulation results are used to systematically analyze how the contact angle (θ) and capillary number (Ca) govern displacement morphology, phase connectivity, and residual phase distribution. Furthermore, a capillary‑number–contact‑angle (Ca–θ) phase diagram characterizing the displacement process is established.

       Key findings are summarized as follows: (1) Under gas–water viscosity ratios representative of the reservoir‑formation stage, pore‑scale gas‑driven water displacement exhibits three distinct regimes: capillary fingering, viscous fingering, and a transitional capillary–viscous fingering regime. In the matrix‑pore model, displacement is dominated by capillary fingering due to pore‑throat constrictions and microstructural bottlenecks, resulting in a dispersed and fragmented displacement front. In contrast, displacement in the pore–fracture model is governed by an interconnected fracture network, where capillary forces are substantially weakened, leading to displacement patterns characteristic of viscous fingering. (2) At low Ca, displacement follows the capillary‑fingering regime, and the gas phase predominantly forms a connected flow network after displacement. At high Ca, viscous fingering dominates, generating numerous isolated gas bubbles and yielding poor gas‑phase connectivity. At intermediate Ca, a transitional regime emerges, combining features of both capillary and viscous fingering. (3) The influences of wettability, capillary number, and pore‑structure type on final gas saturation and gas‑phase connectivity differ markedly between the two models. Under identical displacement conditions, the pore–fracture model attains significantly higher gas saturation and superior gas‑phase connectivity compared to the matrix‑pore model. These insights advance the understanding of methane occurrence and migration in deep coal seams and provide a basis for optimizing coal reservoir development strategies.

Keywords:Deep coal;Gas-water two-phase flow;Displacement pattern;Wettability, Capillary number

How to cite: Jin, X. and Chen, Z.: Pore‑Scale Simulation of Methane‑Water Two‑Phase Flow in Deep Coal Seams Using the Volume of Fluid Method, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2800, https://doi.org/10.5194/egusphere-egu26-2800, 2026.

EGU26-2877 | Posters on site | EMRP1.9

Rock Mechanical Parameters Prediction Based on Digital Drilling Cuttings Mineral Logging Data 

Xin Nie, Yulong Hou, and Zhansong Zhang

With the continuous advancement of oil and gas exploration and development, unconventional resources have become a crucial component of national energy strategies. The extraction of resources such as shale oil and gas relies on technologies like horizontal drilling and multi-stage fracturing, where accurate geomechanical parameters are essential for engineering design. Conventional core-based experiments and well-log inversion methods, though reliable, are often costly, time-consuming, and limited in representativeness. Recent progress in digital cutting analysis—using scanning electron microscopy (SEM) and energy dispersive spectroscopy (EDS)—offers a fast, economical, and practical alternative. This study presents a workflow for predicting rock mechanical parameters from the mineral composition and pore structure of cuttings. Site-collected cuttings were characterized via SEM-EDS to analyze morphology, mineralogy, pore networks, and microfractures. Given the high heterogeneity and anisotropy of shale, a composite modeling approach integrating heterogeneous structure theory and equivalent medium models was applied. This included the Reuss and Voigt bounds, Voigt–Reuss–Hill average, Hashin–Shtrikman bounds, Kuster–Toksöz theory, and Gassmann fluid substitution to estimate equivalent static elastic parameters. These were then converted to dynamic parameters using linear regression to ensure consistency with logging data. Results show strong agreement between cutting-derived parameters and well-log inversions. Young’s modulus and Poisson’s ratio errors range from –12.62% to 4.03% and –10.18% to 10.47%, respectively, within acceptable limits. Although minor uncertainties arise from mineral identification and image segmentation, overall trends match well-log data closely. The introduction of a Weakness Index effectively highlights reservoir heterogeneity and correlates well with measured fracture pressures. A strong linear relationship between static and dynamic parameters, particularly Young’s modulus, supports the reliability of the regression-based conversion. This study confirms the feasibility and applicability of digital cuttings for building rock-physics models and predicting mechanical properties in unconventional reservoirs. The method not only aligns with well-log results but also better captures formation heterogeneity. More importantly, it enables real-time, cost-effective mechanical characterization from wellsite cuttings, offering a practical alternative to core- or log-dependent methods. This is particularly valuable in complex wells such as horizontals, where rapid formation evaluation and fracture design are critical. 

How to cite: Nie, X., Hou, Y., and Zhang, Z.: Rock Mechanical Parameters Prediction Based on Digital Drilling Cuttings Mineral Logging Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2877, https://doi.org/10.5194/egusphere-egu26-2877, 2026.

Pyrite is widely developed in shale formations with diverse occurrence morphologies and relatively low contents. However, it exerts a significant impact on the electrical properties of reservoirs and severely restricts the accuracy of reservoir evaluation. Based on computed tomography (CT) scanning technology, combined with mathematical morphology methods and finite element simulation techniques, this study focuses on the coupling relationship between pyrite occurrence states and reservoir resistivity, along with the quantitative calculation method of pyrite content. The results indicate that: (1) The influence of pyrite occurrence morphologies on the electrical conductivity of shale varies remarkably. Dispersed pyrite particles exert a weak interference on reservoir resistivity, and the rock-electrical relationship conforms to Archie's law. In contrast, massive and banded pyrite have a more prominent impact on resistivity, their conductive contribution exceeds that of pore water. This renders the traditional Archie's law inapplicable. Furthermore, under the condition of the same content, banded pyrite exerts the most significant influence on reservoir resistivity. (2) Three parameters, namely the Pyrite Resistivity Ratio (PRR), the Conductive Path Influence Characterization (VPYRZ), and the Pyrite Occurrence Index (PYI), are constructed to quantitatively describe the nonlinear influence of pyrite with different occurrence morphologies on reservoir resistivity. Combined with scanning electron microscopy (SEM) data, the PYI thresholds for different occurrence morphologies are determined as follows: dispersed pyrite (< 7.8623), massive pyrite (7.8632–16.986), and banded pyrite (>16.986). On this basis, a quantitative calculation model for pyrite content is established. (3) The verification results of actual well logs show that the calculated results of the proposed model are in high agreement with the formation element logging data, and the accuracy meets the practical requirements of reservoir evaluation.

How to cite: Liu, Y.: A Study on the Coupling Relationship Between Pyrite Occurrence Morphologies in Shale and Resistivity, and the Quantitative Calculation Method of Its Content Based on Numerical Simulation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2946, https://doi.org/10.5194/egusphere-egu26-2946, 2026.

Mean grain size (Mz) is a key indicator of depositional processes and reservoir quality, yet its continuous characterization is commonly limited by the availability of core or cuttings data. This study presents a new method for predicting Mz from conventional well logs by integrating Complete Ensemble Empirical Mode Decomposition with Adaptive Noise (CEEMDAN) and Principal Component Analysis (PCA). A density–neutron separation parameter is first constructed to capture lithological and grain-framework variations. Multi-scale components sensitive to grain-size changes are then extracted from this parameter using CEEMDAN, and the dominant controlling features are identified through PCA. The resulting model enables continuous Mz prediction along the wellbore. Comparisons with measured data demonstrate that the proposed approach reliably captures vertical grain-size variations, providing a practical and robust solution for quantitative grain-size characterization and supporting detailed reservoir analysis and geological modeling.

How to cite: Shen, B., Wang, C., Ma, X., and Sun, K.: Quantitative Inversion of Mean Grain Size from Conventional Well Logs Using Complete Ensemble Empirical Mode Decomposition (CEEMDAN)and Principal Component Analysis(PCA), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3232, https://doi.org/10.5194/egusphere-egu26-3232, 2026.

EGU26-3276 | Orals | EMRP1.9

Direct Prediction of Oil Saturation from NMR T₂ Spectra Using Unsupervised Feature Decoupling and Deep Learning 

Qihui Li, Changsheng Wang, Xinmin Ge, Ruiqiang Chi, Yanmei Wang, Wenjing Zhang, Quansheng Miao, and Junsan Zhang

Nuclear magnetic resonance (NMR) T2 spectra provide pore-scale information on fluid occurrence and mobility and are widely used for saturation evaluation. However, in shale and other unconventional reservoirs, strong heterogeneity, multi-fluid signal overlap, and weak/complex relaxation responses often undermine the reliability of conventional cutoff- and template-based saturation methods.

To address this challenge, we propose a data-driven workflow that directly predicts oil saturation from NMR T2 spectra by integrating feature engineering, unsupervised decoupling, and a compact deep-learning regressor. The method first applies robust preprocessing to suppress abnormal values and outliers, followed by dimensionality reduction to extract the most informative latent features. To alleviate multi-component signal superposition, an unsupervised clustering step is introduced to partition spectral patterns into representative groups, providing a more stable feature basis for learning. Finally, a lightweight convolutional neural network (CNN) is employed as the regression model to map processed T2 features to core-calibrated oil saturation, with standard strategies (normalization, dropout/regularization, and learning-rate scheduling) to improve generalization.

The workflow is validated using core-log paired datasets from a shale reservoir, showing that the predicted oil saturation agrees well with laboratory measurements and significantly improves stability compared with conventional interpretation in complex intervals. The proposed approach offers an efficient and scalable route for saturation evaluation in data-limited unconventional plays, supporting sweet-spot identification and development planning.

This research was supported by the National Oil & Gas Major Project (No. 2025ZD1400202) and Natural Science Foundation of Shandong Province, China (No. ZR2023YQ034).

How to cite: Li, Q., Wang, C., Ge, X., Chi, R., Wang, Y., Zhang, W., Miao, Q., and Zhang, J.: Direct Prediction of Oil Saturation from NMR T₂ Spectra Using Unsupervised Feature Decoupling and Deep Learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3276, https://doi.org/10.5194/egusphere-egu26-3276, 2026.

EGU26-3394 | ECS | Orals | EMRP1.9

Electrical Imaging–Based Statistical Indicators for Fracture Identification in Shale-Oil Reservoirs 

Ziming Wang, Xinmin Ge, Long Jiang, Hongxia Sun, Zhongxin Li, Diandong Zhang, and Donggen Yang

Electrical imaging logs are widely used for the quantitative characterization of unconventional reservoirs. However, their applicability is severely limited in pervasively fractured continental shale-oil reservoirs due to strong heterogeneity and complex resistivity responses.

To address this limitation, an electrical statistical framework is developed that integrates variogram-based attributes with smoothness functions to identify fracture occurrence and quantitatively characterize fracture development in shale reservoirs. Resistivity percentile curves derived from electrical imaging logs are analyzed using a moving-window scheme to extract multidimensional parameters, including variance, Shannon entropy, variogram metrics, and smoothness indices. These parameters are jointly used to construct a fracture development index. In addition, fracture-prone intervals are identified using an adaptive thresholding approach constrained by geological rules and resistivity separation characteristics. To suppress the influence of stratigraphic background trends, a local background-resistivity normalization is applied, enabling fracture classification based on resistivity ratios.

The method is validated using shale-oil reservoirs of the Shahejie Formation in the Dongying Sag, eastern China. The results demonstrate that, within a tolerance range of 0.125 m, fracture identification derived from electrical image logs achieves an 85.4% agreement with core descriptions. The identification accuracies for high-conductivity and high-resistivity fractures reach 90.41% and 80.65%, respectively, while approximately 47% of the identified fractures exhibit high conductivity.The proposed approach provides new insights into fracture-filling properties and their vertical distribution, highlighting its applicability to shale-oil reservoir characterization, sweet-spot evaluation, and hydraulic fracturing design. 

This research was supported by the National Oil & Gas Major Project (No. 2024ZD1405102).

Fig. 1. Electrical Imaging–Based Statistical Indicators for Fracture Identification in Well FY3

How to cite: Wang, Z., Ge, X., Jiang, L., Sun, H., Li, Z., Zhang, D., and Yang, D.: Electrical Imaging–Based Statistical Indicators for Fracture Identification in Shale-Oil Reservoirs, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3394, https://doi.org/10.5194/egusphere-egu26-3394, 2026.

Extra-deep electromagnetic (EM) logging-while-drilling (LWD), with its deep investigation and sensitivity to resistivity distribution, is widely used in high-angle and horizontal wells. Due to the complex tool responses of extra-deep EM LWD in heterogeneous formations, eyeball evaluation is often insufficient for accurate bed boundary identification. Therefore, quantitative formation parameter estimation necessitates inversion, with multi-boundary inversion based on 1D models being the most prevalent approach. The inherent limitation of 1D-based inversion is its inability to accurately resolve structurally complex formations, frequently producing oversimplified results. 2D inversion methods alleviate this oversimplification, but their high computational cost limits applicability in real-time geosteering.

In paper, we propose a 1D-2D adaptive parametric inversion framework to combine the efficiency of 1D inversion with the accuracy of 2D inversion. First, we investigate the tool responses and parameter sensitivities in 2D formations using a 2.5D finite-difference algorithm. Then, a scenario-dependent adaptive parametric inversion strategy is developed for specific models based on the sensitivity analysis. For instance, in a fold model, we use a 1D horizontally layered inversion for gently dipping limb regions and a three-point parameterization scheme for the fold core. To improve global optimization, a probabilistic inversion method is established based on the PT-MCMC algorithm, incorporating multiple prior distributions and multiple joint constraints. Finally, the method is applied to the inversion of fold and fault models. Numerical experiments demonstrate that the proposed method accurately reconstructs fold cores and fault structures. Specifically, the relative errors of fault dip angle and fault throw are less than 10%, while the relative error of the fold core location is less than 8%.

Generally, the proposed 1D-2D adaptive parametric inversion framework provides an efficient and robust strategy for real-time geosteering in horizontal and highly deviated wells within complex reservoirs, showing potential for refined reservoir characterization.
We are indebted to the financial support from the National Natural Science Foundation of China (42304140).

How to cite: Chang, J. and Wu, Z.: An Efficient 1D-2D Adaptive Parametric Inversion Method for Extra-Deep Electromagnetic LWD in Complex Scenarios, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3483, https://doi.org/10.5194/egusphere-egu26-3483, 2026.

EGU26-3653 | Orals | EMRP1.9

AI-Driven Automatic Segmentation and Quantitative Characterization of Shale Microstructures 

Xinglei Huang, Yuhang Guo, Xiao Li, and Ying Li

Shale microstructure is critical for predicting shale-oil “sweet spots” and improving reservoir evaluation. As a typical unconventional reservoir, shale exhibits ultra-low permeability, complex pore systems, strong heterogeneity, and diverse mineral compositions with highly uneven spatial distributions; pore morphology and connectivity, together with mineral assemblages, strongly control fluid migration, mechanical behaviour, and acoustic–electrical responses. However, conventional rock-physics experiments and image-analysis workflows are often time-consuming and insufficiently accurate for such complex materials. Here we develop a multi-scale, multi-modal segmentation workflow based on nnU-Net v2. Using paired 0.3 µm-resolution SEM and QEMSCAN images, we perform multi-class segmentation of pores, organic matter, clays, felsic minerals, carbonates, and heavy metal-bearing minerals, achieving a weighted Dice score of 0.95 and clearly outperforming threshold-based segmentation. The SEM-trained network is then transferred to 0.3 µm CT data to enable cross-modality prediction and reconstruct three-dimensional distributions of the segmented phases. We further extend the model to 4 nm-resolution CT images for cross-scale and cross-modality segmentation; three denoising filters are evaluated to suppress noise and improve nanoscale segmentation accuracy. Finally, we compare 3D digital rock volumes generated from single-direction inference with those obtained by tri-axial inference and fusion, highlighting differences in volumetric consistency and structural representation. This workflow provides a robust basis for future multi-scale digital rock construction and for simulations of porosity, permeability, and saturation, thereby supporting more comprehensive shale-oil reservoir assessment.

How to cite: Huang, X., Guo, Y., Li, X., and Li, Y.: AI-Driven Automatic Segmentation and Quantitative Characterization of Shale Microstructures, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3653, https://doi.org/10.5194/egusphere-egu26-3653, 2026.

EGU26-3739 | ECS | Posters on site | EMRP1.9

An Integrated Method for Quantifying Karst Volume in Carbonate Reservoirs 

Jue Hou and Yepeng Yang

The accurate quantification of karst volume is essential for evaluating storage capacity and fluid flow behavior in carbonate reservoirs, which are often highly heterogeneous due to complex diagenetic and karstification processes. However, conventional approaches to karst characterization frequently rely on qualitative descriptions or isolated datasets, lacking an integrated framework that effectively combines petrophysical properties with lithological controls. To address this gap, this study proposes a novel and practical workflow that systematically integrates routine well logs and core data to quantitatively estimate karst-dominated porosity in carbonate sequences. The methodology is designed to be both log-based and scalable, making it suitable for field-wide application even in data-constrained environments.

The proposed method is structured into four sequential and interpretative steps: (1) Data Integration and Quality Control: Multi-source data—including conventional well logs, core measurements, geological models, and lithology logs—are carefully depth-matched and subjected to rigorous quality checks to ensure consistency and reliability. Special attention is paid to correcting for borehole environmental effects and log normalization across multiple wells. (2) Definition of Karst Porosity Threshold: Based on systematic analysis of core-derived porosity-permeability cross-plots, a porosity value greater than 15% is established as a robust indicator for significant karst development. This threshold effectively distinguishes karst-related pore space from matrix porosity and is validated through thin-section and CT-scan observations. (3) Identification of Host Lithology: Lithofacies modeling and petrographic analysis are employed to confirm that karst features are predominantly hosted within dolomite intervals, highlighting the lithological control on karst distribution. Log-based facies classification is calibrated with core data to ensure accurate lithology discrimination in non-cored sections. (4) Calculation of Karst Volume Percentage: The proportion of karst volume is quantitatively computed as the ratio of high-porosity (>15%) dolomite volume to the total pore volume, which includes matrix pores, vugs, and fractures. This volumetric approach enables a more realistic representation of karst contribution to total porosity and reservoir performance.

This workflow was applied to a carbonate reservoir in the Pre-Caspian Basin, where it yielded a karst volume proportion of 11.1%. This result aligns closely with independent core statistics and regional geological understanding, validating the method’s accuracy and applicability. Sensitivity analyses were conducted on the porosity threshold, confirming that the selected 15% cutoff optimally balances discrimination capability and geological plausibility. The integrated approach not only enhances the reliability of karst assessment but also offers a scalable and reproducible tool for reservoir characterization. It supports improved geological modeling, reservoir performance prediction, and development planning in complex carbonate settings, ultimately contributing to more efficient hydrocarbon recovery. Future work will focus on extending the workflow to incorporate seismic attributes and dynamic production data for enhanced 3D karst modeling.

Keywords: Karst Volume; Carbonate; Well Logging; Porosity; Integrated Workflow

How to cite: Hou, J. and Yang, Y.: An Integrated Method for Quantifying Karst Volume in Carbonate Reservoirs, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3739, https://doi.org/10.5194/egusphere-egu26-3739, 2026.

EGU26-4177 | Posters on site | EMRP1.9

Acoustic Remote Detection Logging for Heterogeneous Reservoirs 

Han Wang, Yuhang Guo, Zhitao Zhang, Ziang Ye, and He Sun

Acoustic Remote Detection Logging can extend the investigation range of conventional borehole logging from the immediate vicinity of the borehole to several meters and even tens of meters, providing complementary information for formation evaluation in reservoirs with heterogeneity such as fracture–cavity systems and thin interbeds. Such complex anomalous bodies may reduce the effectiveness of conventional rock-physics log interpretation. Overall, the current work still faces two main issues: the lack of geology-constrained 3D models and the lack of more efficient and transferable interpretation tools, which makes it difficult to establish a stable relationship between complicated reflected wavefields and subsurface heterogeneity.

This study focuses on Acoustic Remote Detection Logging and develops geology-constrained 3D heterogeneous modeling and response analysis. First, a 3D stochastic medium is generated using the spectral synthesis method to produce correlated random fields, which are then mapped to elastic-parameter perturbation fields. Then, a bisection-based thresholding scheme is applied to satisfy a target volume fraction (or porosity), and local-maximum detection is used to determine seed points and spatial distributions for cavities, enabling 3D construction of fracture–cavity heterogeneity. Cavity geometry and scale parameters are constrained by statistical characteristics derived from existing geological and logging data. Finally, CUDA-based parallelization is introduced to improve the efficiency of full 3D model generation and support rapid construction of high-resolution reservoir models.

Based on forward simulations of Acoustic Remote Detection Logging responses excited by dipole shear-wave sources, we design parameter combinations covering formation porosity and fracture–cavity geometric parameters, and summarize the results into response charts/templates for interpretation. These charts provide quantitative relationships between fracture parameters and key waveform features, supporting comparative identification and interpretation of fracture development, orientation, and spatial position under different geological scenarios. In addition, we explore using a model for feature discrimination under chart-based constraints, thereby providing auxiliary support for comparative evaluation and interpretation of fracture parameters.

How to cite: Wang, H., Guo, Y., Zhang, Z., Ye, Z., and Sun, H.: Acoustic Remote Detection Logging for Heterogeneous Reservoirs, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4177, https://doi.org/10.5194/egusphere-egu26-4177, 2026.

EGU26-4225 | ECS | Posters on site | EMRP1.9

Direct Fractal Characterization of Shale Hydrocarbon Content from NMR T1-T2 Echo Train Data 

Mingxuan Gu, Liang Wang, Pengda Shi, Gang Li, and Yizhuo Ai

Accurate estimation of hydrocarbon content is a critical component of shale reservoir evaluation. Although nuclear magnetic resonance (NMR) T1-T2 measurements are highly sensitive to fluid properties, conventional assessments of hydrocarbon content typically rely on empirical interpretation charts or supplementary experiments, which limit their quantitative reliability and practical applicability. In this study, we propose a novel fractal characterization method based on NMR T1-T2 measurements for quantitative evaluation of hydrocarbon content in shale reservoirs. To mitigate the uncertainty introduced by T1-T2 spectral inversion, fractal parameters are directly extracted from the original NMR echo train data, bypassing the inversion process entirely. Numerical simulations demonstrate that the echo-based fractal parameters exhibit significantly enhanced sensitivity and discrimination capability with respect to hydrocarbon content when compared with fractal parameters derived from inverted T1-T2 spectra. Core-scale experiments further validate that the proposed fractal dimension effectively differentiates movable hydrocarbons from pyrolytic hydrocarbons in shale formations. The proposed method provides a robust, efficient, and inversion-independent approach for shale hydrocarbon content evaluation, offering strong potential for both laboratory studies and field-scale NMR applications.

How to cite: Gu, M., Wang, L., Shi, P., Li, G., and Ai, Y.: Direct Fractal Characterization of Shale Hydrocarbon Content from NMR T1-T2 Echo Train Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4225, https://doi.org/10.5194/egusphere-egu26-4225, 2026.

Tight sandstone reservoirs are generally characterized by low porosity and permeability, complex pore structures, and ambiguous electrical responses, which significantly limit the applicability of conventional water saturation evaluation models. To address these challenges, this study proposes a physically constrained reinforcement learning–based symbolic regression framework that integrates nuclear magnetic resonance (NMR)–derived pore size distribution information to automatically derive a dynamic Archie water saturation model with explicit physical interpretability.In the proposed approach, pore size distribution features are embedded into the formation factor formulation, enabling a dynamic correction of the classical Archie equation. A policy neural network combined with reinforcement learning is employed to jointly optimize the model structure and parameters, while explicitly enforcing physical constraints such as monotonicity and nonlinear electrical response behavior.Experimental results demonstrate that, compared with the conventional Archie model, the proposed dynamic model achieves a significant improvement in water saturation prediction accuracy for tight sandstone reservoirs, reducing the mean absolute error by approximately 11%. Moreover, the model more effectively captures the influence of pore structure heterogeneity on the relationship between electrical resistivity and water saturation.This study provides a novel water saturation evaluation methodology that combines physical interpretability with data-driven adaptability for tight sandstone reservoirs and offers valuable insights into the intelligent construction of logging interpretation models for complex reservoirs.

How to cite: Liao, W. and Zhao, B.: A Physically Constrained Dynamically Corrected Archie Saturation Model Based on Pore Size Distribution and Its Application to Tight Sandstone Reservoir Evaluation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4245, https://doi.org/10.5194/egusphere-egu26-4245, 2026.

EGU26-4329 | ECS | Orals | EMRP1.9

An NMR EMG-Based Method for Pore Structure Characterization and Permeability Prediction in Carbonate Reservoirs 

Gang Li, Liang Wang, Mingxuan Gu, and Yizhuo Ai

Carbonate reservoirs host substantial hydrocarbon resources; however, their characterization remains challenging due to strong heterogeneity and complex pore systems, which often produce asymmetric and highly multimodal NMR T₂ distributions. These characteristics undermine the applicability and robustness of conventional pore-structure interpretation and permeability models. To overcome these limitations, we propose a novel nuclear magnetic resonance (NMR)-based method that employs an Exponentially Modified Gaussian (EMG) model to quantitatively characterize pore structure and improve permeability estimation. First, the EMG function is used to decompose the measured T₂ distribution into multiple components with clear physical implications, enabling separation and quantification of pore contributions across scales. Second, the EMG-derived characteristic parameters are subsequently incorporated to refine the conventional Schlumberger-Doll Research (SDR) permeability model, thereby accounting for the impact of complex pore geometry on flow capacity. Validation using diverse carbonate samples demonstrates that the EMG model provides accurate and stable fitting of T₂ distributions across varying pore complexity, ranging from unimodal to highly multimodal distributions. Moreover, EMG-informed permeability estimation yields significantly improved accuracy and robustness compared with conventional methods. Overall, the proposed NMR EMG-based method offers a reliable solution for pore-structure characterization and permeability evaluation in complex carbonate reservoirs.

How to cite: Li, G., Wang, L., Gu, M., and Ai, Y.: An NMR EMG-Based Method for Pore Structure Characterization and Permeability Prediction in Carbonate Reservoirs, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4329, https://doi.org/10.5194/egusphere-egu26-4329, 2026.

EGU26-4382 | ECS | Posters on site | EMRP1.9

Research on Dynamic Wellbore Stability Based on Wellbore Seepage 

Xinyu Liu and Jian Xiong

Due to the mutual flow between drilling mud and formation fluid, the pore pressure in the surrounding rock of the wellbore directly affects the rock’s mechanical properties. Since the properties and density of drilling mud are adjusted in real time during drilling operations, wellbore stability is inherently a dynamic process. This study aims to enhance wellbore integrity and reduce drilling accidents by investigating the dynamic characteristics of wellbore stability.

Rock mechanics experiments were conducted to simulate the mechanical properties of rocks under varying pore pressure conditions, yielding the quantitative relationship between pore pressure and rock mechanical behaviors. In conjunction with the radial seepage characteristics around the wellbore at different drilling stages, dynamic fluid-solid coupling simulations of the wellbore were performed based on geomechanical principles, enabling the development of a dynamic wellbore stability prediction method. This method further facilitates the prediction of key parameters such as wellbore collapse period and radial collapse depth.

This dynamic wellbore stability prediction technology was applied to three wells drilled in sandstone formations. It successfully predicted the collapse depth and period under different drilling mud densities and properties, significantly improving drilling efficiency while ensuring wellbore integrity. Compared with static wellbore stability prediction techniques, this technology provides drilling engineers with a richer set of drilling parameters and defines a clear wellbore collapse period, thereby effectively preventing stuck pipe accidents. Comparative drilling tests in the same block and formation layer showed that drilling efficiency increased by 12%, and the stuck pipe accident rate decreased by 27.3%.

This exploratory research demonstrates that wellbore stability in permeable formations during drilling is indeed a dynamic equilibrium process. As drilling mud properties, time, and stress conditions change, wellbore stability evolves accordingly. Predicting dynamic parameters can provide valuable references for drilling design and optimization, thereby enhancing wellbore integrity and minimizing drilling accidents.

How to cite: Liu, X. and Xiong, J.: Research on Dynamic Wellbore Stability Based on Wellbore Seepage, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4382, https://doi.org/10.5194/egusphere-egu26-4382, 2026.

Identification of fluid components and reliable saturation evaluation remain critical challenges in shale exploration and development. Conventional core experimental methods are often limited by high costs and long cycle times, while laboratory nuclear magnetic resonance (NMR) techniques fail to perform rapid and continuous measurements.  In this study, we propose a rock-constrained multilevel Gaussian mixture model (GMM) approach for the quantitative evaluation of multiple fluids in shale using wellsite NMR data. The proposed workflow begins with normalization and thresholding of the T₁–T₂ spectra. A rock-physics constraint is then incorporated to partition the relaxation domain and distinguish movable fluids from bound fluids. GMM clustering is first applied independently within each relaxation region to extract representative fluid signatures. These characteristic signatures are subsequently integrated into a second-stage GMM analysis, enabling robust identification and quantitative evaluation of individual fluid components. Application to representative shale NMR datasets, coupled with multi-state core experiments, demonstrates that the proposed method effectively identifies multiple fluid components, including heavy components, bound oil, and movable oil. Furthermore, the saturation of various hydrocarbon components can be quantitatively predicted, demonstrating strong agreement with Rock-Eval measurements. The proposed approach provides a practical and reliable solution for rapid downhole fluid identification and saturation evaluation in shale reservoirs.

How to cite: Shi, P., Wang, L., and Gu, M.: A Rock-Constrained Multilevel GMM Approach for Wellsite NMR Multifluid Quantitative Evaluation in Shale, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4645, https://doi.org/10.5194/egusphere-egu26-4645, 2026.

EGU26-4758 | ECS | Orals | EMRP1.9

A New Uncertainty Quantification Method for Petrophysical Parameters Based on NMR Relaxation Spectra  

Yongjie Zhao, Jiangfeng Guo, Qiaosheng Wan, and Ranhong Xie

    Reservoir porosity, permeability, and saturation are regarded as the core parameters in oil and gas exploration. The prediction of reservoir productivity and the analysis of fluid transport behavior in porous media are directly influenced by these parameters. Nuclear magnetic resonance (NMR) is recognized as a non-invasive, non-destructive, and highly quantitative technique. Typically, echo signals are inverted to obtain relaxation spectra, which is then used to calculate rock parameters.

    In the existing methods, reservoir petrophysical parameters are usually calculated based on a relaxation spectrum obtained from a single inversion. However, the inversion of NMR relaxation spectra is inherently an ill-posed problem. Its solutions are characterized by non-uniqueness and high sensitivity to noise. In the traditional interpretation workflows, the single relaxation spectrum obtained from inversion is often assumed to be accurate and deterministic. Consequently, the propagation effect of inversion errors in the calculation of petrophysical parameters is ignored. This leads to a lack of credibility assessment for results in evaluations involving low signal-to-noise ratio (SNR) or unconventional reservoirs.

    To address this challenge, an improved Bootstrap resampling method is proposed in this study. It aims to achieve uncertainty quantification from NMR relaxation spectra to petrophysical parameters. The traditional approach of seeking a single solution is abandoned. Instead, single-measurement echo data are resampled multiple times to generate statistically significant pseudo-sample sets by fully mining the statistical fluctuation information hidden within the single measurement. Subsequently, each set of samples is inverted independently to construct a distribution set of relaxation spectra.

    By performing independent parameter calculations on the relaxation spectrum set, the distribution range, central tendency, and dispersion of each parameter can be obtained. Thus, the impact of data noise and pore size distribution differences on parameter estimation is revealed. On this basis, an error propagation model from the spectral domain to the parameter domain is established. Confidence intervals (CI) and prediction intervals (PI) for porosity, permeability, and saturation are calculated simultaneously. Specifically, model uncertainty caused by the non-uniqueness of the inversion algorithm is primarily quantified by the CI. Meanwhile, data uncertainty resulting from measurement noise is further incorporated into the PI, which provides a broader parameter interval range. A transition from "point estimation" to "interval estimation" for key petrophysical parameters is achieved by this method. Consequently, the robustness and credibility of parameter evaluation under complex reservoir conditions are significantly enhanced.

    This work was supported by the National Natural Science Foundation of China (42304118), the Frontier Interdisciplinary Exploration Research Program of China University of Petroleum Beijing (2462024XKQY009), the Young Elite Scientist Sponsorship Program by BAST (BYESS2023027).

How to cite: Zhao, Y., Guo, J., Wan, Q., and Xie, R.: A New Uncertainty Quantification Method for Petrophysical Parameters Based on NMR Relaxation Spectra , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4758, https://doi.org/10.5194/egusphere-egu26-4758, 2026.

EGU26-6040 | Posters on site | EMRP1.9

Lithology identification of intrusive rocks based on petrochemical big data 

Zhou Quan and the Quan Zhou

To address the high cost and low efficiency of lithology identification for intrusive rocks in oil and gas exploration, this study proposes a hierarchical identification method based on petrochemical big data and machine learning. By integrating global geochemical databases, a standardized sample set covering ultramafic to felsic intrusive rocks was constructed, and a three-level classification system (“group–subgroup–specific lithology”) was established. Visual discrimination charts and an automatic identification model were developed using Linear Discriminant Analysis and Multilayer Perceptron, respectively. The results show that the method achieves over 90% accuracy in the first- and second-level classifications, effectively identifying major rock types such as gabbro, diorite, and granite. Although the accuracy fluctuates in the third-level classification due to compositional overlap and data quality issues, the method exhibits good interpretability and generalizability. This approach provides a low-cost and efficient technical solution for rapid lithology identification and reservoir evaluation, demonstrating potential application in deep and unconventional hydrocarbon exploration.

How to cite: Quan, Z. and the Quan Zhou: Lithology identification of intrusive rocks based on petrochemical big data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6040, https://doi.org/10.5194/egusphere-egu26-6040, 2026.

The accurate petrophysical characterization of unconventional reservoirs, particularly deeply buried fractured–vuggy carbonate systems, remains challenging due to extreme heterogeneity, ultra-low permeability, and strong scale dependency of reservoir properties. Conventional formation evaluation workflows often fail to reconcile geological observations at the core scale with log- and seismic-scale petrophysical interpretations in a physically consistent manner.In this study, we propose an integrated geological–geophysical petrophysical characterization workflow that links core and thin-section observations, electrofacies classification, and seismic data through an electrofacies-constrained seismic waveform-guided inversion framework. Rock types identified from core and petrographic analyses are translated into electrofacies at the log scale to represent pore-structure variability. Electrofacies are incorporated as conditional constraints in a Bayesian seismic waveform-guided porosity inversion framework. Electrofacies-dependent porosity priors derived from well-log statistics restrict the admissible pore-structure space, while seismic waveform similarity controls the lateral propagation of high-frequency porosity features, implicitly embedding seismic facies within the inversion.The resulting porosity volume exhibits enhanced vertical resolution and improved lateral continuity, allowing thin-layer and non-layered heterogeneities to be resolved beyond the limitations of conventional impedance-based inversion. Recognizing that permeability is not directly observable at the seismic scale, permeability is subsequently derived from the inverted porosity volume under electrofacies control, ensuring that pore connectivity and flow characteristics are consistently represented at the appropriate scale.This workflow establishes a causally consistent and scalable solution for advanced petrophysical characterization and formation evaluation of heterogeneous unconventional reservoirs. By integrating geological constraints with seismic waveform-driven inversion, the proposed method effectively bridges core-, log-, and seismic-scale information and demonstrates strong potential for application in complex carbonate systems as well as other unconventional plays.

How to cite: Zhao, A., Tian, F., and Cao, W.: Multi-Scale Petrophysical Modeling and Characterization of Heterogeneous Carbonate Reservoirs Based on Facies-Constrained Seismic Waveform Integration, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6054, https://doi.org/10.5194/egusphere-egu26-6054, 2026.

EGU26-6308 | Orals | EMRP1.9

Response Mechanism of Multi-scale Electrical Logging in Fractured Formations 

Sinan Fang, Zhansong Zhang, Chong Zhang, Xin Nie, Hongwei Song, and Bin Zhao

Fracture parameters play a crucial role in productivity prediction, reservoir evaluation and fracturing production of buried-hill reservoirs and carbonate reservoirs. The main method for calculating fracture parameters is electrical logging based on rock-electric experiments. However, due to significant differences in observation systems between rock-electrical experiments and various electrical logging methods, directly calibrating electrical logging data with cores in different fractured formations will lead to large errors. Based on the finite element method calibrated with core samples, we established micro-fractured formation models and conducted fracture parameter simulation experiments for plunger core samples, full-diameter core samples, electrical imaging logging, micro-spherical focusing logging, shallow lateral logging, and deep lateral logging, respectively, aiming at the influence of multiple fracture parameters. A comparison of the measurement results of the six models for the same fractured formation showed that the fracture-induced resistivity reduction rates were ranked in descending order as follows: electrical imaging logging, plunger core testing, micro-spherical focusing logging, full-diameter core testing, shallow lateral logging, and deep lateral logging, with the maximum discrepancy in resistivity reduction rates across these models reaching a factor of 45. Specifically, the resistivity reduction rate of plunger cores was 2.7 times higher than that of full-diameter cores, and the rate of electrical imaging logging was 11.8 times higher than that of micro-spherical focusing logging, whereas the values for shallow lateral logging and deep lateral logging were identical. Finally, this study proposed a correction rate required for fracture core calibration, which could comprehensively optimize the interpretation range of various resistivity logging methods and effectively improve the interpretation accuracy of reservoirs.

How to cite: Fang, S., Zhang, Z., Zhang, C., Nie, X., Song, H., and Zhao, B.: Response Mechanism of Multi-scale Electrical Logging in Fractured Formations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6308, https://doi.org/10.5194/egusphere-egu26-6308, 2026.

Fluids in porous rocks can be divided into two categories according to their distribution patterns: irreducible fluids and movable fluids. Due to the influence of various geological processes, porous rocks exhibit a wide range of pore size distributions, leading to complex fluid distributions in pores of different sizes. The microscopic distributions of irreducible and movable fluids, namely the contents of irreducible and movable fluids in rock pores of varying sizes, can directly reflect the petrophysical properties of rocks, such as microscopic pore structure characteristics and seepage capacity. In the exploration and development of oil and gas resources, the quantitative characterization of the distributions of irreducible and movable fluids in reservoirs—especially the characterization of movable fluid distributions—is of great significance for reservoir evaluation, productivity prediction, and efficient reservoir development. However, owing to the limitations of actual core data, traditional modeling methods face bottlenecks at the data-driven level, posing challenges to the establishment of accurate fluid distribution characterization models. In this study, the fluid distribution laws in tight sandstones were first analyzed based on core experimental data. Then, the Generative Adversarial Networks (GAN) were used to expand the core dataset. The results of core data processing indicated that the fluid distribution laws of the generated data were consistent with those of the original data, which verified the effectiveness of the adopted data expansion method. Finally, the fluid distribution prediction model were established based on a Multilayer Perceptron (MLP) and realized the accurate characterization of the distributions of irreducible and movable fluids in tight sandstone reservoirs through core experiments and logging data processing.

How to cite: Jin, G., Qin, S., Ma, Y., and Jin, B.: Research on Fluid Distribution Characterization Method of Tight Sandstone Reservoirs Based on Machine Learning Using Nuclear Magnetic Resonance Logging, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6375, https://doi.org/10.5194/egusphere-egu26-6375, 2026.

EGU26-6994 | Orals | EMRP1.9 | Highlight

Multi-scale Fracture Evaluation Method for Shale Reservoirs in Deep Formation Wufeng-Longmaxi in Southern Sichuan 

Yufeng Xiao, Hongyan Wang, Xinmin Ge, Gaojie Xiao, Shuangquan Chen, Zhoutuo Wei, and zhenxue Jiang

The fractures in the deep shale reservoirs in southern Sichuan are one of the main factors affecting the enrichment of shale gas, fracturing design, and development effectiveness. Therefore, it is necessary to carry out multi-scale joint inversion methods to identify and evaluate fractures at different scales to improve the accuracy of their evaluation and prediction.

To address the above problems, four different scale fracture evaluation methods and their consistency studies have been conducted, including core, logging, remote detection, and seismic. Through the analysis of geological characteristics, core observation, CT scanning and experiments on acoustic anisotropy, the intervals of shale fractures and their anisotropic characteristics are determined. The anisotropy coefficient of shale reservoirs is calculated by dipole cross-wave logging, determining the longitudinal development degree and characteristics of shale reservoir fractures. The acoustic field imaging is used to extract the reflection coefficients of high and low frequency Stoneley wave and equivalent anisotropic coefficients of shear reflection waves, which allowed for the identification and evaluation of the development characteristics and effectiveness of fractures near borehole at a remote acoustic detection scale. Based on high-resolution seismic data with wide azimuth vector offset, the pre-stack seismic anisotropy coefficient is constructed, clarifying the intrinsic relationships between the fracture medium reservoir parameters described at four different scales.

The study shows that the deep shale reservoir fractures of Wufeng-Longmaxi Formation in southern Sichuan are mainly bedding fractures, mostly in a closed state, followed by structural fractures, most of which are filled with calcite. The high-and low-frequency Stoneley wave reflection coefficients in the formations Wufeng-Long11 of the first deep shale gas evaluation well Lu203 in southern Sichuan, show a significant difference, with fracture development and good reservoir connectivity, with an initial production of 1.38×106m3/d. Determining the acoustic anisotropy coefficient is a common parameter for evaluating shale reservoir fractures from core scale to seismic scale, and innovating the acoustic remote detection of shear wave reflection waves equivalent anisotropic coefficients fills the gap in detection range and resolution from logging to seismic scale, achieving high precision prediction of small-scale fractures of 3-20m. The results are generally consistent with core, logging, acoustic remote detection imaging, gas testing results, and production performance, proving the effectiveness of the multi-scale fracture evaluation method of shale reservoirs using cross-scale constraints. Further predictions indicate that the well area Lu 203 is characterized by the development of small fractures/bedding fractures on the basis of relatively stable structures, while the well area Yang101 is the development of structural fractures on the basis of large fault, with multiple calcite fillings, which is one of the main factors contributing to the significant differences in shale gas production between the above two areas. The proposed multi-scale fracture evaluation method based on acoustic anisotropy coefficients provides significant reference value for the comprehensive evaluation of unconventional reservoir fractures.

This research was supported by the National Oil & Gas Major Project (No. 2025ZD1403902) and the CNPC International Science and Technology Cooperation Project (No. 2023DQ0422).

Fig. 1  AVAZ inversion plan along the O3w layer in L203 Block in Southern Sichuan

How to cite: Xiao, Y., Wang, H., Ge, X., Xiao, G., Chen, S., Wei, Z., and Jiang, Z.: Multi-scale Fracture Evaluation Method for Shale Reservoirs in Deep Formation Wufeng-Longmaxi in Southern Sichuan, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6994, https://doi.org/10.5194/egusphere-egu26-6994, 2026.

EGU26-7042 | ECS | Posters on site | EMRP1.9

Deep Learning–Based 3D Multi-Mineral Digital Rock Modeling and Diagenetic Simulation 

Zijie Lu, Kelai Xi, and Yuqi Wu

The construction of three-dimensional multi-mineral digital rock cores is essential for the fine characterization of reservoir pore–throat structures and for the quantitative evaluation of reservoir electrical, acoustic, and mechanical properties.Existing digital rock core modeling approaches can be broadly classified into physical experimental methods and numerical reconstruction methods.Physical experimental methods can produce relatively realistic three-dimensional digital rock cores; however, they are costly and struggle to achieve fine mineral discrimination.Numerical reconstruction methods offer advantages such as low cost and high efficiency; however, most high-fidelity approaches remain limited to single-mineral digital rock cores, whereas multi-mineral modeling methods often rely on idealized assumptions.To address these limitations, this study proposes a 2D–3DGAN-based deep learning algorithm capable of generating three-dimensional multi-mineral digital rock cores from a single AMICS image.Using the “AMICS + 2D–3DGAN” modeling framework, three-dimensional multi-mineral digital rock cores are constructed with high accuracy, efficiency, and realistic multi-mineral representation.The accuracy of the generated results is systematically evaluated by analyzing diagenetic characteristics and by comparing the generated cores with training images in terms of mineral content, pore size distribution, and two-point correlation functions.The results demonstrate that the proposed method significantly enhances reconstruction accuracy and generation efficiency while maintaining economic feasibility, thereby providing a solid foundation for subsequent simulations of multi-mineral diagenetic evolution and reservoir property analysis.Previous studies on diagenesis have largely relied on qualitative approaches, such as identifying diagenetic evolution sequences and constructing two-dimensional schematic representations.Based on the generated three-dimensional multi-mineral digital rock cores, this study proposes a “nucleation–growth” algorithm for numerically simulating diagenetic processes, enabling quantitative modeling of diverse cementation morphologies that closely reflect geological conditions.Meanwhile, the four-parameter structure method is improved to quantitatively simulate dissolution and replacement processes with varying morphologies and to control the precipitation location of dissolution by-products, either inside or outside dissolution pores.Ultimately, a three-dimensional digital rock core diagenetic evolution model based on diagenetic sequences is established, enabling analysis of the evolution of reservoir properties—such as porosity, permeability, tortuosity, and coordination number—through diagenetic processes.

How to cite: Lu, Z., Xi, K., and Wu, Y.: Deep Learning–Based 3D Multi-Mineral Digital Rock Modeling and Diagenetic Simulation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7042, https://doi.org/10.5194/egusphere-egu26-7042, 2026.

EGU26-7276 | ECS | Orals | EMRP1.9

Research on Non-intrusive Detection of Marine Sediment Cores Using Magnetic Induction Tomography 

Chenxin Yuan, Changchun Zou, and Cheng Peng

The physical characterization of marine sediment cores is pivotal for the exploration of shallow seafloor resources, such as gas hydrates and shallow gas. While non-intrusive imaging is essential for preserving sample integrity, conventional detection methods face significant limitations. Although X-ray CT offers high-resolution imaging, its application is constrained by bulky instrumentation and time-consuming scanning processes, rendering it impractical for rapid, on-site evaluation of sediment cores. Conversely, Electrical Resistivity Tomography (ERT) offers high sensitivity to electrical properties but relies on contact measurements. This inevitably disturbs the original structure of unconsolidated sediments and suffers from electrode polarization, thereby degrading imaging quality.

To address these challenges, this study investigates a non-intrusive imaging technique based on Magnetic Induction Tomography (MIT) to probe the internal electrical conductivity structure of sediments. In this method, excitation coils surrounding the core are energized with time-harmonic alternating current to generate a primary magnetic field. According to the principle of electromagnetic induction, eddy currents are induced within the conductive sediment, subsequently generating a secondary magnetic field that opposes the primary one. Since the intensity and path of these eddy currents are strictly governed by the spatial distribution of conductivity within the core, the internal structural information can be retrieved by detecting the perturbed total magnetic field via an array of receiver coils.

The feasibility of this proposed method was validated through forward modeling based on the Finite Element Method. To reconstruct the conductivity distribution from the magnetic measurements, the inverse problem was solved using the Gauss-Newton method. Preliminary simulation results demonstrate that the magnetic induction-based approach can effectively recover the internal electrical structure of the target, confirming its potential as a compact and efficient tool for marine sediment characterization.

This work was supported by the National Natural Science Foundation of China, Grant No. 42274232.

How to cite: Yuan, C., Zou, C., and Peng, C.: Research on Non-intrusive Detection of Marine Sediment Cores Using Magnetic Induction Tomography, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7276, https://doi.org/10.5194/egusphere-egu26-7276, 2026.

Electromagnetic logging while drilling (EM LWD) provides unique capabilities for both look-around and look-ahead detection, making it a foundational technology for identifying formation interfaces in complex horizontal and ultra-deep well applications. Over recent decades, its detection depth has advanced from a few meters to a remarkable range of several tens of meters. Nevertheless, directional EM LWD remains the primary geosteering method in horizontal wells, largely due to its sensitivity to formation boundaries and relatively low operational cost. In early directional EM LWD applications, where the maximum detection range was generally below 5 meters, one-dimensional (1D) formation models were widely adopted for forward simulation and inversion. However, current-generation tools can achieve detection ranges approaching ten meters, meaning that formation influences now extend across a significantly larger volume. Continuing to use conventional 1D models under such conditions may introduce substantial errors. While transitioning to two-dimensional (2D) models preserves accuracy, the increased model dimensionality substantially reduces computational speed, hindering real-time inversion.

In this paper, we propose an approximate method for simulating directional EM LWD responses in 2D models, designed to address this inherent trade-off between computational efficiency and accuracy. The core concept involves reducing complex 2D geological models into a series of 1D representations, which are then solved using a pseudo-analytical algorithm. First, the computational domain is divided into sliding windows of varying widths, defined with reference to the tool’s depth of investigation. Within each window, curved formation interfaces are approximated by straight lines to construct a 1D model, from which the tool response is computed. The series of 1D responses is then synthesized to obtain an approximate response for the original 2D model. To ensure both efficiency and reliability, an automated workflow integrating progressive model reduction with real-time quality control is implemented. The process begins with a coarse 1D approximation (typically 3–5 models). A divergence metric quantifies its representativeness; if below a preset threshold, the result is accepted. Otherwise, an iterative refinement phase is activated, dynamically increasing the number of 1D models only where necessary until the synthesized response stabilizes. The algorithm was validated on representative fault and fold models. Numerical results demonstrate that the proposed method successfully avoids the oversimplification inherent in conventional 1D modeling while achieving a computational speedup of more than 10 times compared to conventional full 2D numerical simulations.

We are indebted to the financial support from the National Natural Science Foundation of China (42304140).

How to cite: Wu, Z. and Yue, X.: An Efficient Method for Approximating Directional Electromagnetic LWD Responses in Complex 2D Formation Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8555, https://doi.org/10.5194/egusphere-egu26-8555, 2026.

EGU26-8628 | ECS | Posters on site | EMRP1.9

Fracture Identification in Electrical Image Logs with Limited Samples by Incorporating Outcrop Priors 

Yizhuo Ai, Liang Wang, Mingxuan Gu, Li Gang, Pengda Shi, and Ziling Zhao

Micro-resistivity imaging logging is one of the primary techniques for subsurface fracture identification. However, conventional manual interpretation is time-consuming and highly subjective, while existing deep learning-based methods generally require large-scale, well-annotated datasets, resulting in substantial labeling costs and limited applicability in data-scarce scenarios. To address these challenges, this study proposes a fracture identification method for electrical image logs under limited-sample conditions by incorporating prior knowledge derived from outcrop fractures. Leveraging the morphological and statistical similarities between surface outcrop fractures and subsurface electrical image responses, a two-stage training strategy based on a Multi-scale Attention Network (MANet) backbone is developed. In the first stage, optical images of outcrop fractures are preprocessed through grayscale transformation and noise injection to approximate the feature distribution of electrical image logs, enabling the network to learn generalizable edge and texture features. In the second stage, outcrop–electrical image pairs with similar fracture morphology and texture characteristics are generated through similarity matching, and the model is fine-tuned using a composite loss function incorporating Correlation Alignment (CORAL), thereby accelerating domain adaptation to subsurface logging environments. Experimental results from basement reservoirs in the Dongping area of the Qaidam Basin demonstrate that the proposed method significantly improves fracture identification performance under limited-sample conditions. Compared with baseline models, the proposed approach achieves improvements of 13.05% in accuracy and 12.88% in Intersection over Union (IoU), reaching 81.13% and 75.74%, respectively. These results indicate that the proposed method effectively alleviates data scarcity issues in electrical image log interpretation and provides robust technical support for fracture characterization and hydrocarbon resource evaluation.

How to cite: Ai, Y., Wang, L., Gu, M., Gang, L., Shi, P., and Zhao, Z.: Fracture Identification in Electrical Image Logs with Limited Samples by Incorporating Outcrop Priors, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8628, https://doi.org/10.5194/egusphere-egu26-8628, 2026.

As the fundamental constituent units of hybrid shale oil reservoirs, laminae exhibit complex structures and diverse combination types, leading to strong reservoir heterogeneity. Therefore, revealing the structural characteristics of laminae and their controlling mechanisms is crucial for understanding the storage and occurrence properties of such reservoirs. This study focuses on the shale reservoirs of the Fengcheng Formation in Mabei, Xinjiang, integrating methods such as cast thin sections, field emission scanning electron microscopy (FE-SEM), X-ray diffraction (XRD), and nitrogen adsorption to characterize the storage properties of laminae. On this basis, laser scanning confocal microscopy was used to accurately analyze the oil-bearing properties and occurrence differences within individual laminae. Furthermore, nuclear magnetic resonance (NMR) technology was applied to elucidate the controlling effects of complex laminae combinations on storage and occurrence. The results indicate that: (1) The Fengcheng Formation contains diverse laminae types, including felsic clastic laminae, tuff laminae, dolomite laminae, limestone laminae, siliceous laminae, borax laminae, and organic matter laminae. (2) The primary storage spaces consist of dissolution pores in felsic clastic/tuff laminae, intragranular and intercrystalline pores in dolomite laminae, and intercrystalline pores in limestone/siliceous/borax laminae. Strong dissolution, conducive to the development of high-quality reservoirs, occurs when the proportion of felsic clastic laminae is 50%-60% or dolomite laminae is 20%-40%. (3) Confocal microscopy characterization reveals that dolomite, micritic siliceous, and felsic clastic laminae exhibit superior oil-bearing properties. The differences in oil-bearing properties are mainly controlled by two key factors: ① The interbedded distribution of source and reservoir rocks without barriers; the closer a lamina is to the source, the better its oil-bearing properties. ② A coordinated source-to-reservoir ratio; the optimal oil-bearing properties occur when the ratio of source laminae to reservoir laminae is 1:3 to 2:1, with the poorest properties when the ratio exceeds 6:1. NMR core-scale testing further validates these controlling patterns. The conclusion is that the key to efficient storage and occurrence of shale oil lies in the optimal spatial configuration and coordinated proportion between high-quality source rocks and effective reservoirs.

How to cite: Wang, H.: Research on the Control Mechanism of Mixed-Type Shale Laminar Structure on Shale Oil Reservoir and Storage Properties, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8636, https://doi.org/10.5194/egusphere-egu26-8636, 2026.

EGU26-8697 | Posters on site | EMRP1.9

A DNN–LSTM–GPC framework for TOC prediction in marine shales of the X Block using multi-source logging data 

Xinmin Ge, Ziming Wang, Chuanliang He, Xiang Ge, Jingyu Fan, Xiaoguang Wu, Donggen Yang, and Cheng Zhai

Marine shales of X-block are featured with poor organic matter, over maturity and complex mineralogical assemblages, which collectively result in weak organic-related logging responses. As a consequence, conventional total organic carbon (TOC) evaluation methods exhibit substantial uncertainties associated with baseline calibration and parameter generalization, thereby limiting prediction accuracy and robustness.

To overcome these limitations, this study develops a physics-constrained deep learning framework for TOC prediction that integrates multi-source logging data using a hybrid DNN–LSTM–GPC architecture. High-resolution nuclear magnetic resonance (NMR) and electrical imaging logs are incorporated as primary data sources to extract multi-scale, organic-matter-sensitive features. These features are further integrated with conventional well logs to construct a comprehensive feature space that captures organic matter distribution, pore structure characteristics, and lithological variability. In addition, an improved ΔLogR model and region-specific rock-physics constraints are embedded within the deep learning framework to ensure physical consistency and geological interpretability.

Application results demonstrate that the proposed method achieves superior prediction performance in low–organic-matter marine shales, yielding a root mean square error of 0.08% and a coefficient of determination (R²) of 0.95. The model consistently outperforms multivariate regression, uranium-based approaches, and porosity-difference methods, while maintaining stable predictive capability in intervals exhibiting pronounced TOC heterogeneity. These results indicate that physics-constrained deep learning integrated with multi-source logging data provides a reliable and effective approach for micro-scale TOC evaluation and favorable reservoir identification in low–organic-matter marine shale systems.

This research was supported by the Natural Science Foundation of Shandong Province of China (ZR2023YQ034) and Shida Jingwei Industry-Education Integration Research Institute Project (15572259-25-ZC0607-0011).

Fig. 1. Comparison of total organic carbon (TOC) prediction results for marine shale in Well JY6, X Block, obtained from different methods.

How to cite: Ge, X., Wang, Z., He, C., Ge, X., Fan, J., Wu, X., Yang, D., and Zhai, C.: A DNN–LSTM–GPC framework for TOC prediction in marine shales of the X Block using multi-source logging data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8697, https://doi.org/10.5194/egusphere-egu26-8697, 2026.

The fluid inclusion homogenization temperature method is the most widely used approach for reconstructing hydrocarbon accumulation history in deep to ultra-deep carbonate rocks. However, there are three major limitations: (1) The difficulty in restoring the eroded thickness of target strata, leading to uncertainty in the reconstruction of tectonic and burial history. (2) It is common to use the brine inclusion homogenization temperature as a substitute for hydrocarbon inclusion trapping temperature. However, it is often challenging to find coexisting hydrocarbon and brine inclusions within the same host mineral. (3) It is difficult to determine the trapping time based on the trapping temperature. As in multi-cycle superimposed basins, the same trapping temperature may correspond to multiple ages on the tectonic-burial history curve, resulting in non-unique solutions.

The application of laser U-Pb isotopic dating of carbonate minerals and clumped isotope thermometry has addressed these limitations and led to the development of a new method for reconstructing hydrocarbon accumulation history in deep to ultra-deep carbonate reservoirs. (1) Restoration of the eroded thickness of strata is achieved through multi-phase diagenetic mineral age-temperature constraints, effectively resolving the uncertainty in the tectonic-burial history reconstruction. (2) Direct measurement of hydrocarbon inclusion trapping temperature, overcoming the challenge of determining trapping temperature when no coexisting brine inclusions are present in the host mineral. (3) Direct measurement of hydrocarbon inclusion trapping time, addressing the issue of non-uniqueness in accumulation ages for multi-cycle superimposed basins.

This method has been applied to reconstruct the accumulation history of natural gas reservoirs in the Dengying Formation of the Sichuan Basin. It has significantly higher accuracy and success rates compared to the fluid inclusion homogenization temperature method.

How to cite: Anping, H. and Anjiang, S.: A New Method for Reconstructing Hydrocarbon Accumulation History of Deep to Ultra-Deep Carbonate Reservoirs, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8804, https://doi.org/10.5194/egusphere-egu26-8804, 2026.

Shale oil and gas, as typical unconventional resources, have become crucial for stabilizing oil and gas production in China. The calculation of shale reservoir fracturability index is a core step in evaluating engineering sweet spots. However, acoustic logging data of shale formations are susceptible to geological interfaces, borehole deviation, and particularly the bedded structure-induced anisotropy. Such anisotropy causes the measured acoustic interval transit time to deviate from the true formation value, leading to inaccurate in-situ stress calculation and thus compromising the reliability of fracturability evaluation. Accurate acquisition of formation AIT is essential for optimizing fracturing schemes and analyzing borehole stability.

To address this issue, a correction method for acoustic anisotropy of bedded shale in horizontal wells was established. Based on the bedded shale medium model assumption, the formation stiffness coefficients and elastic wave velocities were derived using the equivalent medium theory and elastic wave equation. Shale models with varying bedding angles were constructed to analyze the functional relationships between acoustic velocity, acoustic anisotropy coefficient, and bedding angle.

Numerical simulation results demonstrate that the acoustic interval transit time of bedded shale exhibits significant anisotropic characteristics: both acoustic interval transit time and acoustic anisotropy coefficient increase with the increase of bedding angle, and the acoustic anisotropy coefficient has a good power exponential relationship with the cosine of the bedding angle. A correction model for acoustic anisotropy of bedded shale was thus developed. Field application in horizontal wells of Block L showed that after correction, the peak of the normal distribution curve of acoustic interval transit time in the target reservoir of horizontal wells was highly consistent with that of pilot wells. The corrected acoustic interval transit time was used to calculate Poisson's ratio, Young's modulus, horizontal principal stress difference, and fracture pressure, further deriving the fracturability index. Comparison with the fracturability index calculated from core experimental data indicated that the average relative error of the results was reduced by 9.28%.

This study provides a reliable acoustic anisotropy correction method for bedded shale, which is of great significance for improving the accuracy of shale reservoir fracturability evaluation and guiding the identification of engineering sweet spots.

How to cite: Wu, B. and Zhao, J.: Correction of Acoustic Anisotropy of Bedded Shale and Its Application in Fracturability Evaluation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9050, https://doi.org/10.5194/egusphere-egu26-9050, 2026.

The effective development of unconventional shale oil reservoirs depends on the accurate prediction of seepage pathways. In the lacustrine shales of the upper submember of the fourth member of the Shahejie Formation (Es4U) in the Dongying Sag, bedding fractures serve as both primary storage spaces and critical fluid conduits. However, intense reservoir heterogeneity makes it challenging to reliably identify fracture-prone intervals using well-log responses alone.

Based on systematic core descriptions and fracture statistics from research wells, this study integrates thin-section petrography, X-ray diffraction (XRD), total organic carbon (TOC) analysis, and logging data to perform a multi-scale correlation of bedding fracture occurrences.

The results demonstrate that: (1) bedding fractures are diagenetic products triggered by clay mineral dehydration/transformation and hydrocarbon-induced overpressure; (2) the development of these fractures is synergistically governed by carbonate and clay mineral contents, organic matter abundance, and lamina density, with laminated clay-rich lithofacies identified as the dominant zones for fracture occurrence.Building upon these geological insights, a vertical development model for bedding fractures was established to provide quantitative geological constraints for logging evaluation. By utilizing conventional logging suites (e.g., integrating AC, GR, and DEN curves), intervals characterized by carbonate content of 20%–60%, clay content of 20%–35%, TOC > 2%, and well-developed laminated structures are identified as potential fracture-bearing zones.

This model effectively bridges geological genesis with logging attributes, providing a direct geological foundation for the prediction of favorable seepage pathways in shale reservoirs using borehole geophysical data.

How to cite: Liu, C., Wang, G., and Yin, Z.: Geological Patterns and Conventional Well-log Prediction of Bedding Fractures in Lacustrine Shales: A Case Study from the Upper Submember of the 4th Member of the Shahejie Formation, Dongying Sag, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10363, https://doi.org/10.5194/egusphere-egu26-10363, 2026.

EGU26-11545 | ECS | Posters on site | EMRP1.9

Bayesian-Optimized XGBoost for High-Precision Lithofacies Identification in Carbonate Reservoirs Using Geophysical Well Logs 

Jingyu Yang, Liang Wang, Mingxuan Gu, Yizhuo Ai, and Gang Li

Carbonate reservoirs possess substantial hydrocarbon resource potential and have become a major focus of exploration in recent years. However, the complex geological settings, pronounced lithological heterogeneity, and strong vertical variability of carbonate reservoirs pose significant challenges to conventional lithofacies identification methods. Such approaches are often time-consuming, highly subjective, and limited in their ability to accurately discriminate complex lithofacies assemblages, thereby constraining the efficient development of carbonate reservoirs. Geophysical well logging offers advantages such as low acquisition cost, continuous coverage, and high vertical resolution, making it a fundamental dataset for continuous lithofacies characterization. In this study, integrated geological information, including whole-rock analysis, petrographic thin sections, and scanning electron microscopy, is employed to systematically investigate the mineral compositions and pore structure characteristics of different lithofacies, and the corresponding logging response mechanisms are quantitatively investigated. Five conventional logging curves—gamma ray, acoustic, neutron porosity, bulk density, and resistivity—are selected to construct a multidimensional feature parameter set. Considering the differences in numerical ranges among logging curves and the imbalance in lithofacies sample distributions, data normalization and class imbalance correction are performed prior to model training. Subsequently, a high-precision lithofacies identification model based on conventional well logs is developed by integrating Bayesian optimization with the Extreme Gradient Boosting (XGBoost) algorithm. The results indicate that the predicted lithofacies are highly consistent with geological interpretations, core observations, and thin-section identifications, demonstrating that the Bayesian-optimized XGBoost model exhibits robust classification performance and effectively captures the complex nonlinear relationships between lithofacies and logging responses. Compared with traditional machine learning methods, the proposed approach achieves significantly improved identification accuracy, providing robust technical support and a reliable theoretical foundation for carbonate reservoir evaluation and hydrocarbon exploration.

How to cite: Yang, J., Wang, L., Gu, M., Ai, Y., and Li, G.: Bayesian-Optimized XGBoost for High-Precision Lithofacies Identification in Carbonate Reservoirs Using Geophysical Well Logs, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11545, https://doi.org/10.5194/egusphere-egu26-11545, 2026.

Shales exhibit significant seismic anisotropy, which can cause errors in seismic imaging, seismic attribute analyses and reservoir characterization. During deposition and burial, platy clay mineral particles tend to align along bedding planes, creating distinct direction-dependent seismic properties — a primary cause of anisotropy. Therefore, investigating the influence of clay on the evolution of shale anisotropy during compaction is crucial for enhancing seismic interpretation accuracy. However, quartz, serving as the primary rigid grain in shales, complicates this process. It forms a resisting framework that interferes with the preferred orientation of clay platelets. Hence, solely studying pure clay is insufficient, and investigating the compaction behavior of clay-quartz mixtures is of great value to accurately characterize the evolution of seismic anisotropy in realistic shale environments. Given their dominance in shale mineralogy, kaolinite and illite were chosen as the representative clay end-members for our study. We prepared eight clay-quartz mixtures (4 kaolinite-quartz mixtures and 4 illite-quartz mixtures) by mixing different amounts of clay and quartz: 100%, 80%, 60% and 40% of clay by weight. To simulate the natural burial process, these water-saturated loose sediments were subjected to uniaxial mechanical compaction experiments.

Experimental results indicate that for both groups, porosity decreases monotonically while seismic anisotropy increases with increasing compaction stress. However, the influence of quartz content differs significantly between the two mineral systems. In the kaolinite group, Thomsen parameters ε and γ show a negative correlation with quartz content at identical pressure levels. The illite group, conversely, exhibits more complex behavior: while γ remains negatively correlated with quartz fraction, ε displays a non-monotonic trend—initially decreasing, then increasing, and finally decreasing again as quartz content rises. Furthermore, the parameter δ serves as a distinct discriminator: kaolinite mixtures exhibit suppressed δ values (near zero or negative), whereas illite mixtures consistently display positive δ values (> 0.10), indicative of well-stratified compliant bedding.

These findings underscore that the "bridging effect" of quartz and the resulting anisotropy are strictly controlled by clay mineralogy. Specifically, the high positive δ of illite implies that conventional elliptical assumptions may cause significant errors in processing. Therefore, accurate seismic interpretation requires mineral-specific anisotropic models that account for the distinct structural evolution of kaolinite and illite during compaction.

Fig. 1 Thomsen’s anisotropy parameters ε, γ, and δ versus porosity for the K-series and I-series samples.

How to cite: Guo, X. and Han, T.: Evolution of Anisotropic Acoustic Properties in Clay-Quartz Mixtures during Mechanical Compaction: Implications for Shale Burial, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11711, https://doi.org/10.5194/egusphere-egu26-11711, 2026.

EGU26-15374 | Orals | EMRP1.9

esearch on roduction rofile evaluation method for shale gas wells based on distributed Fiber-Optic Temperature Sensing (DTS) 

Hongwei Song, Tie Xia, Mingxing Wang, Haitao Huang, Zhansong Zhang, Sinan Fang, Xin Nie, Bin Zhao, and Chong Zhang

Aiming at the challenge of achieving full-wellbore continuous monitoring and quantitative evaluation of shale gas well production profiles, this study develops an evaluation method based on distributed fiber-optic temperature sensing (DTS). By comprehensively considering the effects of fluid thermal convection in the wellbore, wellbore-formation heat exchange, and the Joule-Thomson effect on wellbore temperature distribution, a forward model of wellbore fluid temperature is established to accurately characterize the depth-dependent temperature distribution of the wellbore. On this basis, with model parameters as inversion variables, a squared error objective function between DTS-measured temperatures and forward-calculated temperatures is constructed, and the Bayesian inversion method is employed to solve the key parameters of the production profile, realizing the quantitative inversion of gas-water two-phase production for each producing layer. Field verification is conducted using an actual shale gas well: results show that the average absolute error between forward-calculated temperatures and DTS-measured temperatures is 0.05°C, indicating a high overall profile agreement; the gas and water two-phase production obtained by inversion is consistent with the on-site production dynamic recognition law, verifying the accuracy and reliability of the proposed method. This research provides effective technical support for the engineering application of DTS technology in production dynamic monitoring and development optimization of shale gas wells.

How to cite: Song, H., Xia, T., Wang, M., Huang, H., Zhang, Z., Fang, S., Nie, X., Zhao, B., and Zhang, C.: esearch on roduction rofile evaluation method for shale gas wells based on distributed Fiber-Optic Temperature Sensing (DTS), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15374, https://doi.org/10.5194/egusphere-egu26-15374, 2026.

EGU26-15411 | ECS | Posters on site | EMRP1.9

Research on the Influence of NMR Acquisition Parameters on Fluid Distribution in Shale Reservoirs 

Jier Zhao, Bing Xie, Yuexiang Wang, and Li Bai

Unconventional reservoirs are confronted with numerous challenges due to their complex pore structures and diverse fluid occurrence states; therefore, the accurate acquisition of pore structure characteristics and fluid property parameters has become the key factor restricting development efficiency. 2D nuclear magnetic resonance (NMR) logging obtains more observation information by introducing longitudinal relaxation time (T1), and it exhibits good application effects in wettability evaluation, reservoir parameter calculation and fluid property identification .The factors affecting NMR relaxation signals are multivariate, mainly including pore fluid properties (viscosity, density, etc.), pore structure characteristics (pore size and distribution, pore connectivity, etc.), magnetic susceptibility differences between rocks and fluids, and the content and distribution of paramagnetic minerals. The coupling of these factors complicates the mapping relationship between relaxation signals and reservoir properties, which urgently requires in-depth analysis.In the field of shale oil exploration and development, there are various types of 2D NMR instruments, and significant differences exist in their observation methods, measurement sequences and acquisition parameters, which further pose challenges to the cross-scale characterization and comprehensive interpretation of reservoir parameters. Therefore, this study analyzes the influencing factors of acquisition parameters on NMR from both experimental and numerical simulation scales.The influence of instrument frequency on 2D NMR is investigated through experiments, and the effects of echo spacing, waiting time and number of echoes on NMR measurement and inversion results are studied via numerical simulation. This research further clarifies the influence of acquisition parameters on fluid distribution characterized by 2D NMR, and verifies the reliability of NMR logging interpretation data in shale reservoirs.

How to cite: Zhao, J., Xie, B., Wang, Y., and Bai, L.: Research on the Influence of NMR Acquisition Parameters on Fluid Distribution in Shale Reservoirs, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15411, https://doi.org/10.5194/egusphere-egu26-15411, 2026.

Currently, researchers at home and abroad mainly study the pore space of marine shale, so the research on the pore space of marine-transitional shale is still relatively small. Based on the research findings, marine-continental transitional shale exhibits wide distribution, significant resource potential, and promising exploration and development prospects. This paper addressed this gap by analyzing the geochemical characteristics, petrological features, and pore characteristics of shale in the Upper Permian Leping Formation of the Sichuan Basin. It has been obtained through experimental analysis that the shale's reservoir storage space primarily consisted of organic pores, providing significant potential for shale gas accumulation. The gas adsorption experiments demonstrated the development of micropores, which contributed substantially to the pore specific surface area and volume in Leping shales. Additionally, the TOC content and clay minerals in shale samples have an influence on the storage space of shale. The TOC content had a more significant correlation with micropore volume and specific surface area, and clay mineral content had a better correlation with pore volume and specific surface area of mesopores and macropores. Furthermore, the calculated fractal dimensions (D1, D2, and D3) for the Leping Formation ranged from 2.3616 to 2.5832 (average: 2.4835), 2.7698 to 2.8654 (average: 2.8172), and 2.3274 to 2.5161 (average: 2.4287), respectively. These values indicate that the pores have a complexity and heterogeneous. D1 and D2 are mainly affected by clay minerals, indicating that the complexity of mesopores is mainly controlled by clay minerals; D3 is mainly controlled by TOC content, indicating that the complexity of micropores is mainly controlled by TOC content.D3 has a good positive correlation with pore characterization parameter, indicating that the pore will be more complex with the increase of micropores' percentage and its volume and surface area.The findings from this study provide valuable insights into the pore characteristics of marine-continental transitional shale and offer potential implications for exploration and development prospects in the area.

How to cite: xiao, S. and Fu, X.: The pore characteristics and fractal characteristics of Permian marine-continental transitional shales in the Sichuan Basin, southwestern China, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15446, https://doi.org/10.5194/egusphere-egu26-15446, 2026.

Look-ahead electromagnetic logging while drilling (EM LWD) technology has been widely used in geostopping due to its capability to characterize resistivity distributions ahead of the bit. However, a complex nonlinear relationship between tool responses and rock properties makes it difficult to image the geological structure. Therefore, inversion is essential to reconstruct resistivity distributions and determine formation boundary positions. Currently, gradient-based and artificial intelligence algorithms are commonly used for look-ahead inversion and have shown considerable potential. However, most related studies have focused on the analysis of tool detection capabilities, while research regarding inversion applicability and thin-layer formations remain insufficiently addressed. Additionally, due to the weak signal contribution from the area ahead of the drill bit, challenges still remain, such as the high tendency of inversion to fall into local optima and strong dependence on tool configuration.

In this paper, a look-ahead inversion framework based on the Levenberg-Marquardt (LM) algorithm is proposed, and its applicability to layered formation inversion is investigated. To prevent the inversion from being trapped in local optima, a continuous random multi-initial-value search strategy is proposed. Specifically, formation resistivity from look-around detection is used as a constraint, and random perturbations are applied to parameters to be inverted to select multiple initial values. Furthermore, the look-ahead signal decay is closely associated with tool configuration. By optimizing the selection of response curves through the adjustment of coil frequencies and transmitter-receiver spacings, the accuracy of the look-ahead inversion is further improved. Results demonstrate that the proposed inversion framework achieves an accuracy of up to 80% in the inversion of the distance to the nearest boundary for layered formations and yields favorable results in thin and multi-layer formations. It also provides algorithmic support for look-ahead EM LWD inversion and lays a theoretical foundation for further research on look-ahead inversion in formations with complex structures.

We are indebted to the financial support from the National Natural Science Foundation of China (42304140).

How to cite: Xiao, H., Cheng, C., and Wu, Z.: An LM Algorithm-Based Inversion and Applicability Analysis for Look-Ahead Electromagnetic Logging While Drilling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15621, https://doi.org/10.5194/egusphere-egu26-15621, 2026.

EGU26-15708 | Posters on site | EMRP1.9

A Method for Characterizing Pore Structure of Gas-Bearing Sandstone Based on Nuclear Magnetic Resonance 

Bing Xie, benjian zhang, qingshong tang, xun zhu, jier zhao, yuexiang wang, li bai, and qiang lai

Tight sandstone reservoirs are generally characterized by low porosity, low permeability, and complex pore structures, which pose significant challenges to reservoir evaluation. Nuclear Magnetic Resonance (NMR) T2 spectra can characterize pore structures and fluid states in porous media. Therefore, gas-displacing-water petrophysical experiments were carried out to investigate the variations of T2 spectra under different saturation states.The study finds that the T2 spectrum in the original state presents a multi-peak distribution dominated by long relaxation components. With the increase of gas saturation, the macropore peak value decreases and the porosity tends to decrease. Meanwhile, compared with the gas-bearing state, the macropore peak widens when the core is water-saturated. Analysis shows that this phenomenon is caused by the low hydrogen index of gas.Thus, a spectrum correction model for gas-bearing sandstone reservoirs was established based on the Gaussian distribution, which corrects the T2 spectrum morphology and porosity components to their original states. After gas saturation correction, the T2 spectrum mainly presents a bimodal distribution dominated by short relaxation components. The irreducible water saturation calculated from the corrected T2 spectrum is more consistent with the core measurement results.Combined with NMR experiments, this study clarifies the NMR response mechanism of reservoirs under different saturation states, establishes a Gaussian distribution model for T2 spectrum correction of gas-bearing sandstone, and ultimately achieves accurate characterization of pore structures.

How to cite: Xie, B., zhang, B., tang, Q., zhu, X., zhao, J., wang, Y., bai, L., and lai, Q.: A Method for Characterizing Pore Structure of Gas-Bearing Sandstone Based on Nuclear Magnetic Resonance, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15708, https://doi.org/10.5194/egusphere-egu26-15708, 2026.

EGU26-16220 | Posters on site | EMRP1.9

Development and Application of a Rock Physics Model to Infer Pore-Geometry and Clay-Distribution in Argillaceous Sandstone 

Bing Wang, Xingyao Yin, Zhengqian Ma, and Kun Li

Due to its favorable pore-permeability characteristics, sandstone serves a crucial role in applications such as oil and gas production, freshwater extraction, and underground CO₂ storage. As the primary reservoir space and migration pathway for hydrocarbons, accurate porosity data are essential for seismic exploration and reservoir development. In unconventional reservoirs, establishing an appropriate tight sandstone rock physics model is key to understanding how petrophysical parameters influence porosity and permeability. However, conventional models often fail to dequately represent both the three-dimensional irregularity of pore geometries and the spatial distribution of clay minerals.

To address these limitations, this study develops a novel rock physics model that incorporates superspherical pores and clay distribution to characterize argillaceous sandstone. Clay is categorized into structural clay (within the matrix) and dispersed clay (within pores). Following a sequential approach that reflects natural sandstone grain stacking, the proposed model is constructed by employing Voigt-Reuss-Hill averaging methods to incorporate structural clay, coupling the superspherical pores model, and applying solid substitution equations to determine the saturated rock modulus, which contains dispersed clay. This framework allows quantitative analysis of how pore geometry and clay occurrence states affect rock elastic properties.

However, in practical settings, the high cost of well logging often prevents direct measurement of these parameters. Therefore, a simulated annealing algorithm is employed to inversely determine pore characteristics and clay content in different occurrence states at each sampling point along the wellbore.

The validity and practical applicability of the proposed model are demonstrated through comprehensive sensitivity analyses and real-data applications.

How to cite: Wang, B., Yin, X., Ma, Z., and Li, K.: Development and Application of a Rock Physics Model to Infer Pore-Geometry and Clay-Distribution in Argillaceous Sandstone, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16220, https://doi.org/10.5194/egusphere-egu26-16220, 2026.

Detecting fluid contacts, such as oil-water interfaces, remains a significant challenge for conventional seismic exploration when the acoustic impedance contrast is weak. However, the seismoelectric effect, which depends on electrical conductivity and electrokinetic coupling, provides a promising method for interface detection. In this study, we investigate the radiating seismoelectric electromagnetic (EM) reflection and transmission coefficients generated at an interface between two fluid-saturated porous media under fast P-wave incidence.

We analytically derive the reflection and transmission coefficients for all generated wave modes (fast P, slow P, SV, and EM waves) using Pride’s theory and Helmholtz decomposition. To verify the validity of our derivation, we calculate the energy fluxes of the wavefields using the electrokinetic Poynting vector and confirm that energy conservation is strictly satisfied.

Analyzing the frequency- and angle-dependent behavior of the reflection and transmission coefficients, we show that seismoelectric conversion is directly governed by the contrast in elastic and electric properties of the reservoir and the fluids therein, at the interface. Building on this, we compare the response of an "elastic interface" (strong mechanical contrast) with an "electric interface" (strong conductivity contrast but weak mechanical contrast, representing an oil-water contact). The analysis shows that while the seismic reflection energy at the electric interface is negligible, the reflected seismoelectric EM wave energy is comparable to the seismic signal generated at a strong lithological interface. These findings suggest that reflected seismoelectric waves are a reliable tool for identifying oil-water interfaces that are effectively invisible to conventional seismic surveys.

How to cite: Liu, Y. and Smeulders, D.: Seismoelectric Radiating Reflection and Transmission at Porous–Porous Interfaces: Angle- and Frequency-Dependent Coefficients, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17981, https://doi.org/10.5194/egusphere-egu26-17981, 2026.

EGU26-21370 | ECS | Posters on site | EMRP1.9

A novel method for quantitative characterization of organic matter based on NMR FID acquisition mode 

Chenyu Xu, Ranhong Xie, Jiangfeng Guo, Xiangyu Wang, and Gong Zhang

Continental shale oil reservoirs in China are abundant in Solid Organic Matter (SOM), which represents a significant potential hydrocarbon resource. Nuclear Magnetic Resonance (NMR) is an effective tool for evaluating shale oil reservoirs. However, restricted by instrument dead time, it is difficult for the conventional CPMG acquisition mode to capture signals from ultra-short relaxation components such as SOM.To address this, this work introduces the Free Induction Decay (FID) acquisition mode, proposing two novel quantification workflows based on FID signal integration and a direct T1-T2* spectrum, respectively. These approaches are designed to effectively capture the ultra-short components that are typically missed by standard CPMG sequences.The proposed methodology was validated against comprehensive geochemical benchmarks. The results demonstrate that the FID-driven approach yields a superior correlation with geochemical data compared to conventional methods. It exhibits high statistical consistency with Step-by-Step (SBS) Rock-Eval pyrolysis data, proving its capability to accurately quantify total solid hydrogen content, including solid petroleum hydrocarbons, bitumen, and kerogen. This work provides a non-destructive and high-precision means for evaluating the resource potential of shale oil reservoirs.

How to cite: Xu, C., Xie, R., Guo, J., Wang, X., and Zhang, G.: A novel method for quantitative characterization of organic matter based on NMR FID acquisition mode, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21370, https://doi.org/10.5194/egusphere-egu26-21370, 2026.

EGU26-1431 | ECS | Posters on site | GD3.1

Flow through a slab tear? Lateral variations in seismic anisotropy beneath the Colombian Andes 

Christopher Carchedi, Lara Wagner, and Gaspar Monsalve

Slab tears are observed around the globe with increasing frequency as datasets and imaging methodologies improve, though the interactions between slab tears and the surrounding mantle flow remain enigmatic. Constraints on mantle flow around and through slab tears are crucial to a comprehensive understanding of slab-mantle interactions, as (1) cross-tear flow may allow mixing between upper mantle reservoirs otherwise separated by subducting slabs, and (2) cross-tear flow may impact the strength of nearby corner flow and therefore influence regional dynamic topography. However, the ability to study slab tears and their impact on mantle flow is limited by the number of slabs with clearly observed tearing and sufficient measurement density to capture lateral variations in mantle flow across the tear. On both counts, the Colombian Andes serve as an ideal region to study the interplay between slab tears and mantle dynamics.

The Colombian Andes are shaped by complex interactions between the subducting Nazca and Caribbean plates, as most clearly manifested by the Caldas Tear—a sharp lateral offset in slab seismicity near 5.5°N spanning more than 150 km. Using data collected across this boundary during the recent MUSICA (Modeling, Uplift, Seismicity, and Igneous geochemistry of the Colombian Andes) broadband seismic deployment, we investigate lateral variations in seismic anisotropy across the Colombian Andes by measuring shear-wave splitting of SKS and SKKS phases from teleseismic earthquakes.

Measurements of shear-wave splitting offer direct observational constraints on seismic anisotropy. Seismic anisotropy in the upper mantle forms primarily from the deformation-induced alignment of intrinsically anisotropic olivine crystals. Under various ambient stress and hydration conditions, different olivine petrofabrics develop that relate the bulk anisotropic fast direction to the orientation of maximum extensional strain. By inferring petrofabric type, shear-wave splitting measurements can directly constrain the geometry of deformation in the upper mantle and thus provide insight into the impact of complex slab geometry on mantle dynamics.

Our findings detail a complex regional pattern of mantle flow as the result of three interacting flow components: (1) entrained trench-perpendicular corner flow in the mantle wedges above sinking plates, (2) mantle flow through the Caldas Tear, and (3) trench-parallel flow far east of both subducting plates. Measured splitting delay times far exceed those expected from lithospheric anisotropy alone and thus support a deeper anisotropic source. Additionally, we observe strong back azimuthal variations in splitting measurement quality and quantity that demand further investigation. Future work will explore constraining lateral and vertical anisotropic complexity simultaneously using splitting intensity tomography.

How to cite: Carchedi, C., Wagner, L., and Monsalve, G.: Flow through a slab tear? Lateral variations in seismic anisotropy beneath the Colombian Andes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1431, https://doi.org/10.5194/egusphere-egu26-1431, 2026.

EGU26-2307 | ECS | Orals | GD3.1

Depth rotations of azimuthal seismic anisotropy associated with relative importance of Couette/Poiseuille flow in the asthenosphere 

Zhirui Ray Wang, Clinton P. Conrad, Sergei Lebedev, Giampiero Iaffaldano, and John R. Hopper

Azimuthal seismic anisotropy in the upper mantle is crucial for understanding the spatial patterns of past and present upper mantle deformation. Traditional interpretation of such anisotropy attributes to relative shear between surface plates and mantle. This requires the orientation of anisotropy azimuths to remain constant with depth. However, inferences of azimuthal anisotropy based on surface wave tomographic models often reveals depth-dependent azimuths. To this end, the existence of mechanically weak, thin asthenosphere beneath the lithosphere facilitates the channelization of plate-driven Couette flow and pressure-driven Poiseuille flow. The combination of two flows, especially when misaligned, yields depth rotations of asthenospheric shear. This provides a geodynamically plausible link between asthenospheric flow properties and depth rotations of azimuthal seismic anisotropy. In this submission, we utilize publicly available azimuthal seismic anisotropy models together with predictions from a global mantle flow model that incorporates Couette/Poiseuille flow. We find that Poiseuille flow profoundly affects depth rotations of seismically inferred azimuthal anisotropy. Prominent depth rotations are under the Atlantic basin and the Nazca plate, where Poiseuille flow dominates the modeled asthenospheric flow regime. Significant Poiseuille flow may exist beneath the Indian basin, yet with small depth rotation, probably because of its directional alignment with Couette flow. Our results indicate that interpretation of azimuthal seismic anisotropy cannot be simply tied to relative shearing between plates and mantle. Instead, the relative importance of Couette and Poiseuille flows must be taken into account.

How to cite: Wang, Z. R., Conrad, C. P., Lebedev, S., Iaffaldano, G., and Hopper, J. R.: Depth rotations of azimuthal seismic anisotropy associated with relative importance of Couette/Poiseuille flow in the asthenosphere, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2307, https://doi.org/10.5194/egusphere-egu26-2307, 2026.

EGU26-3092 | Orals | GD3.1 | Highlight

Seismic anisotropy measurements within AdriaArray: a review of previous and new data 

Silvia Pondrelli, Julia Rewers, Piotr Środa, Katarina Zailac, Josip Stipčević, and Simone Salimbeni

The central Mediterranean area is a place where seismic anisotropy measurements have been collected for years, mainly along the Italian peninsula. Several different techniques have been applied to obtain this information, that carries relevant indications on the state of deformation at depth, both in the Earth’s crust and in the mantle. The most common type of measurements comes from the analysis of shear wave splitting of core phases (*KS), and from splitting intensity measurements. Seismic anisotropy patterns are a major support in answering questions such as where tectonic plates are actively deforming and which processes drive plate deformation. These are some of the questions addressed by the AdriaArray project. The seismic experiment AdriaArray aimed to densify the collection of seismographic data to the east with respect to the Adriatic microplate. The area covered by the project spans from southern France to the Black Sea in longitude and from Central Europe to the central Mediterranean in latitude, reaching the Sicily channel and the Hellenic Trench. Part of this wide area is already well studied for seismic anisotropy, as previously obtained data show. However, AdriaArray acquired data from 950 permanent and temporary broad-band stations thanks to the cooperation of nearly 40 institutions (https://orfeus.readthedocs.io/en/latest/adria_array_main.html) and most of them, located in the eastern part of AdriaArray study region, are now under analysis. Within the project, a Collaborative Research Group dedicated to seismic anisotropy has been created. It is working on building a dataset of shear-wave splitting measurements by improving already produced results with new data. The same has been done with splitting intensity measurements, with ongoing analyses for regions such as Sardinia, the eastern Adriatic coast and further east.

How to cite: Pondrelli, S., Rewers, J., Środa, P., Zailac, K., Stipčević, J., and Salimbeni, S.: Seismic anisotropy measurements within AdriaArray: a review of previous and new data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3092, https://doi.org/10.5194/egusphere-egu26-3092, 2026.

The Slave craton in northwest Canada is characterized by thick, cold, depleted lithosphere, and its surface geology includes some of the oldest rocks on the planet. In addition, the central Slave has proven economic importance, with a thriving diamond industry fed by suites of Miocene kimberlites. Previous studies of Slave craton architecture and anisotropy suggested a stratified lithosphere within the central Slave, likely associated with craton formation processes and subsequent metasomatism.

Since the original shear-wave splitting studies carried out in the central Slave craton, new seismograph installations have been carried out which permit an expanded view of the architecture of the craton as a whole, as well as its margins. Here we measure (or remeasure) shear wave splitting parameters for the complete dataset, which spans up to three decades for the longest-running stations. This systematic approach allows for a comprehensive comparison of anisotropic parameters across the craton.

Preliminary results suggest that NE-SW fast-polarization orientations dominate the craton at a large scale, though with significant local variability in the central Slave, suggesting lateral variability in lithospheric properties. We look for azimuthal variations in splitting measurements that may indicate stratified anisotropy, and we compare the results with models of azimuthal anisotropy from recent surface wave tomography studies.

How to cite: Darbyshire, F. and Dave, R.: Seismic anisotropy in the Slave craton, northern Canada: inferences from a new shear-wave splitting compilation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3197, https://doi.org/10.5194/egusphere-egu26-3197, 2026.

EGU26-3264 | Posters on site | GD3.1

Crustal structural and anisotropy in northeastern Tibetan Plateau from receiver functions 

Ruiqing Zhang and Yixiong Hua

Abstract

Deformation in northern (NE) Tibet is essential for understanding the geodynamic processes of crustal thickening and outward growth associated with the Indo-Asian collision. We analyze receiver function data recorded by the regional seismic array of ChinArray-Ⅱ and permanent stations of the study region. The crustal thickness and Vp/Vs ratio are estimated using the H–κ grid searching technique (Zhu et al., 2000) . We also perform a joint analysis of Pms from radial and tangential receiver functions to measure fast polarization direction and splitting time (Liu et al., 2012). The harmonic analysis is adopted to obtain reliable crustal azimuthal anisotropy (Sun et al., 2012). Our result shows that the crust is significantly thickened (≥50 km) west of ~103°, while the Vp/Vs ratio is relatively low (~1.73) beneath the Qilian orogeny. We also found measurements of crustal azimuthal anisotropy beneath 71 stations in which the Pms arrivals with a dominant degree-2 back azimuth variations. The crustal anisotropy shows a north-south change across the Longshoushan fault. The measured splitting time in the region south of the Longshoushan fault is 0.22-1.02 s (with an average of 0.46 s). The fast direction mainly along the NW direction is roughly close to the fast polarization from XKS (Chang et al., 2021), which is parallel to the trending of the Qian orogenic belt, indicating a vertically coherent lithospheric deformation beneath the NE Tibet. To the north, the Alxa block exhibits a NNE-NE fast polarization with an average delay time of ~0.47s. Such observation differs from the fast-axis direction of mantle anisotropy, indicating that the crust and lithospheric mantle are decoupled. The north-south variation in crustal anisotropy of our study area may suggest that the growth front of the northeastern Tibetan Plateau may have extended to the Longshoushan fault.

 

Acknowledgments

Seismic data of the ChinArray was provided by the International Earthquake Science Data Center at Institute of Geophysics, China Earthquake Administration (https://doi.org/10.11998/ IESDC). Seismic waveforms recorded by the permanent stations of the China National Seismic Networks can be downloaded from the National Earthquake Data Center, China Earthquake Administration (https://data.earthquake.cn/) (Zheng et al., 2010). This research was supported by the NSF of China (42030310, 42474133).

 

References

Zhu, L., & Kanamori, H. 2000. Moho depth variation in southern California from teleseismic receiver functions. J. Geophys. Res., 105(B2), 2969–2980.

Liu H., Niu F., 2012. Estimating crustal seismic anisotropy with a joint analysis of radial and transverse receiver function data. Geophys. J. Int., 188: 144–164.

Sun Y., Niu F., Liu H., et al. 2012. Crustal structure and deformation of the SE Tibetan plateau revealed by receiver function data. Earth Planet. Sci. Lett., 349-350: 186–197.

Chang L., Ding Z., Wang C., 2021. Upper mantle anisotropy and implications beneath the central and western North China and the NE margin of Tibetan Plateau. Chin. J. Geophys. (in Chinese), 64(1):114-130.

How to cite: Zhang, R. and Hua, Y.: Crustal structural and anisotropy in northeastern Tibetan Plateau from receiver functions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3264, https://doi.org/10.5194/egusphere-egu26-3264, 2026.

EGU26-3503 | Posters on site | GD3.1

Singularity points in multi-layered anisotropic medium  

Alexey Stovas

The slowness surfaces for P, S1 and S2 waves in anisotropic medium are defined by solving the Christoffel equation. The regular point on the slowness surface can be mapped on corresponding group velocity surface. The irregular (singularity) point on the slowness surface results in the plane curve in the group velocity domain (Stovas et al., 2024).

The characteristic equations for double and triple singularity points define the tangent cone of second and third order, respectively. If the plane wave passes through singularity points in some layers of multilayered model, the effective characteristic equation has order given by product of orders of characteristic equations from individual layers. Therefore, the order of effective characteristic equation can be computed as N=2K3L, where K and L are the number of layers with double and triple singularity points, respectively. The effective characteristic polynomial FN(Δp1,Δp2,Δp3)  (the N-th order tangential cone) for multi-layered model can be computed by resultant of individual characteristic polynomials,where Δpj,j=1,2,3, are the increments in slowness projections.The number of individual branches is given by J=Floor[(N+1)/2]. The dual curve ΦM (V1,V2,V3)=0 is the group velocity umage of Nth-order singularity point, where M=N(N-1)-2n-3c (Quine, 1982), with n and c being respectively the number of nodes and cusps for curve FN=0. It is shown that the tangential cone does not have cusps (c=0) but can have nodes if N≥6. The inflection points and bitangents for curve FN=0 respectively result in cusps and nodes for dual curve ΦM=0. The cusps affect the Gaussian curvature computed in vicinity of singularity point (Stovas et al., 2025). The irregularities in phase and group domain are illustrated in Figure by dots for two-layer model with double singularity points in both layers (N=4, J=2, n=2 and M=8).

Figure. Two-layer model with double singularity points. a) Curve F4=0 in affine plane (phase domain). Four inflection points on converted wave branch are shown by black dots. Two bitangents are shown by dotted lines limited by gray dots. b) Group velocity image (Φ8=0) of quartic singularity point (dual curve). Four cusps are shown by black dots, and two nodes are shown by gray dots. Solid and dashed lines stand for pure wave modes (S1S1 and S2S2) and converted (S1S2 and S2S1) waves, respectively.

References

Stovas, A., Roganov, Yu., and V. Roganov, 2024, Singularity points and their degeneracies in anisotropic media, Geophysical Journal International 238 (2), 881- 901.

Stovas, A., Roganov, Yu., and V. Roganov, 2025, Gaussian curvature of the slowness surface in vicinity of singularity point in anisotropic media, Geophysical Journal International 240 (3), 1917-1934.                                                                    

Quine, J.R., 1982, A Plücker equation for curves in real projective space, Proceedings of the American Mathematical Society, 85, no.1, 103-107.

How to cite: Stovas, A.: Singularity points in multi-layered anisotropic medium , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3503, https://doi.org/10.5194/egusphere-egu26-3503, 2026.

EGU26-4099 | Orals | GD3.1

Mapping upper-mantle fabric at continental scale: frozen tectonics and active flow patterns in western Canada 

Andrew Frederiksen, Christian Phillips, and Yu Gu

Teleseismic shear-wave splitting is a widely-used technique for measuring oriented fabric in the crust and upper mantle; such fabric is an important marker for current or past deformation. The technique yields both the orientation (fast direction) and cumulative intensity (split time) of the net fabric. However, published splitting results, particularly split times, can have puzzling inconsistencies that make mapping splitting over large areas challenging; semivariograms of compiled splitting results show a lack of spatial coherence in split time measurement when studies using different methods are combined. I present modelling work that demonstrates that these inconsistencies result from an inherent bias in splitting measurement, particularly pronounced for split time, that is sensitive to details of the data processing methods and is amplified by averaging single-event measurements. With a correct choice of averaging method (error-surface stacking), this bias can be mitigated sufficiently to allow split time to be mapped over large areas, as demonstrated using compiled data from western Canada. The results show strong spatially-coherent variations along the strike of the Cordillera, which may represent regions of dominant vertical vs. horizontal flow in the upper mantle, driven by complex Cordilleran active tectonics.

How to cite: Frederiksen, A., Phillips, C., and Gu, Y.: Mapping upper-mantle fabric at continental scale: frozen tectonics and active flow patterns in western Canada, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4099, https://doi.org/10.5194/egusphere-egu26-4099, 2026.

EGU26-4243 | Orals | GD3.1

Subslab flow beneath subduction zones revealed by multiple-layer shear wave splitting inversion 

Ban-Yuan Kuo, Cheng-Chien Peng, and Jean-Paul Montagner

Shear wave splitting is widely used to probe seismic anisotropy, but its depth resolution is limited. Building on the formulation of Silver and Savage (1994), we apply a Bayesian inversion that explicitly accounts for uncertainty in shear-wave polarization orientation (θ) to resolve multilayer anisotropy from splitting parameters. We apply this approach to source-side S and SKS data from the Cocos subduction zone, and to SKS data from station NNA above the South America subduction zone and station SNZO at the southern Hikurangi margin. Subduction in all three regions is shallow to flat, minimizing dip-angle effects on SKS. The inversion yields tightly constrained fast directions for both upper and lower anisotropic layers. Three-layer inversions show progressive rotation with depth consistent with two-layer solutions, but are not required by the data. In the Cocos system, the upper-layer fast direction is unambiguously aligned with Cocos plate motion in the NNR reference frame, consistent with subduction-entrained flow. In contrast, beneath NNA and SNZO, the upper and lower layers exhibit trench-subparallel and trench-normal anisotropy, respectively—opposite in layering sense to the poloidal–toroidal flow structure predicted by dynamic models. If both layers reside in the subslab mantle, the trench-parallel upper layer flow would decouple the deeper mantle from the slab, raising questions about how the apparent subduction-driven flow is maintained at depth. Alternatively, the upper layer may reflect deformation within or above the slab. Possible sources of trench-parallel anisotropy include frozen-in oceanic lithospheric fabrics, trench-parallel mantle-wedge flow, or inherited fabrics related to nearby continental shear zones. These results highlight the complexity of subslab dynamics and demonstrate the value of probabilistic multilayer inversion for interpreting shear-wave splitting.

 

How to cite: Kuo, B.-Y., Peng, C.-C., and Montagner, J.-P.: Subslab flow beneath subduction zones revealed by multiple-layer shear wave splitting inversion, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4243, https://doi.org/10.5194/egusphere-egu26-4243, 2026.

The recent increase in seismic activity in the southern Sichuan Basin has attracted substantial public interest and simultaneously provides an important opportunity to investigate upper crustal anisotropy, which offers key constraints on the regional stress field and crustal deformation. In this study, we obtained 1,845 high-quality local shear-wave splitting measurements from 15 stations, along with 2,027 null measurements from 19 stations. The results reveal a single anisotropic layer characterized by a horizontal symmetry axis at depths of approximately 3–7 km. The fast polarization directions exhibit clear spatial variability, which is primarily controlled by the spatial distribution of earthquakes rather than temporal evolution. Near the Baimazhen Syncline, the fast polarization directions align with the strike of the strata and form a circular pattern around the synclinal core, indicating that the anisotropy in this region is dominantly structure-controlled. In contrast, stations located in the southern Weiyuan Anticline and the western Baimazhen Syncline display fast directions of N171.7°E and N45.9°E, respectively. These orientations are consistent with the P axes derived from earthquake focal mechanisms, suggesting that anisotropy in these areas is primarily governed by the regional stress field. Overall, this study enhances our understanding of the complex geological framework of the southern Sichuan Basin and underscores the need for caution when interpreting potential temporal variations in seismic anisotropy in future investigations. This work was supported by the National Natural Science Foundation of China (Grant 42374124).

How to cite: Qiang, Z., Wu, Q., and Li, Y.: Spatial Heterogeneity of Upper Crustal Anisotropy in the Southern Sichuan Basin (China) Revealed by Local Shear-Wave Splitting, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4419, https://doi.org/10.5194/egusphere-egu26-4419, 2026.

EGU26-4571 | ECS | Posters on site | GD3.1

Seismic anisotropy analysis across Southwestern Australia reveals ENE‐trending lithospheric architecture linked to Archean Yilgarn Craton formation 

Miriam Gauntlett, Caroline Eakin, Nitarani Bishoyi, Ping Zhang, John-Paul O'Donnell, Ruth Murdie, Meghan Miller, Robert Pickle, and Reza Ebrahimi

The southwest region of Western Australia is one of the oldest continental regions on Earth, hosting the Archean Yilgarn Craton, bounded by the Proterozoic Albany-Fraser and Pinjarra orogens. Here we calculate shear wave splitting of the PKS and SKS teleseismic phases using stations from Phases 1 and 2 of the WA Array (average station spacing 40 km), as well as other temporary and permanent networks in the study region. We find evidence for coherent seismic anisotropy, with the regional average delay time (1.24 ± 0.62 s) comparable to the global average, δt = 1 s. Although fast polarization orientations show variation, they are not aligned with current plate motion and the expected asthenospheric flow direction. In the South West Terrane, fast polarization orientations match the trend of ancient structural faults. By contrast, structural faults in the Youanmi Terrane and the Eastern Goldfields Superterrane are oriented at an angle compared to the E–W and NE–SW fast polarizations. Instead, the seismic anisotropy pattern shows a striking similarity to E–W trending Precambrian (2.42 Ga) dykes that extend uninterrupted across the Yilgarn Craton. We propose that lithospheric fabrics frozen-in at the time of craton formation (~2.76–2.65 Ga) generated a mechanical weakness which subsequently influenced the orientation and emplacement of the dykes. Further evidence for a similar, ancient (~2.73 Ga) architectural fabric comes from recent isotope geochemistry analysis of primary ENE-trends within the Yilgarn Craton. Overall, these results point toward large-scale, fossilized lithospheric fabric within the Yilgarn Craton, preserved for over two billion years, offering a unique window into the formation and early evolution of the continent. 

How to cite: Gauntlett, M., Eakin, C., Bishoyi, N., Zhang, P., O'Donnell, J.-P., Murdie, R., Miller, M., Pickle, R., and Ebrahimi, R.: Seismic anisotropy analysis across Southwestern Australia reveals ENE‐trending lithospheric architecture linked to Archean Yilgarn Craton formation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4571, https://doi.org/10.5194/egusphere-egu26-4571, 2026.

EGU26-5755 | Posters on site | GD3.1

Mapping the Ivrea Geophysical Body and its anisotropic properties beneath the Western Alps using receiver functions analysis 

Judith Confal, Silvia Pondrelli, Simone Salimbeni, and Nicola Piana Agostinetti

We constrain the extent and anisotropic properties of the Ivrea Geophysical Body (IGB) beneath the Western Alps using receiver function (RF) analysis of 66 teleseismic datasets. The IGB represents one of the most prominent examples of shallow mantle material within continental crust, yet its geometry, composition, and tectonic significance remain debated beyond its well-known positive gravity anomaly. Using teleseismic waves recorded from temporary seismic deployments and permanent seismic networks across the western Alps, we perform a comprehensive receiver function (RF) analysis that indicates the presence of anisotropic mantle materials at shallow depth, associated with the occurrence of the IGB, in terms of P-to-s converted energy out of the radial plane. We characterise the anisotropic rock volumes solving an inverse problem using a Neighbourhood Algorithm. The results indicate that 35 out of 66 RF data-sets from this study, together with five additional stations from a previous study, display coherent anisotropic characteristics directly above the high-gravity anomaly and can be associated with the IGB. These stations exhibit strong anisotropy (~15%) and a coherent fast-axis pattern that systematically rotates from south to north, following the arcuate geometry of the Alpine trench. The depth distribution of the anisotropic interfaces constrains the IGB as a continuous lithospheric-scale body approximately 170 km long, 30-50 km wide, and 20-45 km thick, with its upper boundary as shallow as 1 km depth. The whole body is slightly dipping towards the East. Seismic velocities and anisotropy magnitudes indicate a dominantly mantle-derived composition, consistent with a peridotitic protolith variably overprinted by serpentinite-rich shear zones. Our results refine the three-dimensional extent of the IGB and demonstrate that its anisotropic fabric records the deformation associated with Alpine subduction, slab rollback, and subsequent exhumation, providing new constraints on the tectonic evolution of the western Alpine lithosphere.

How to cite: Confal, J., Pondrelli, S., Salimbeni, S., and Piana Agostinetti, N.: Mapping the Ivrea Geophysical Body and its anisotropic properties beneath the Western Alps using receiver functions analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5755, https://doi.org/10.5194/egusphere-egu26-5755, 2026.

EGU26-5995 | Orals | GD3.1

Radial anisotropy of the upper mantle 

Sergei Lebedev, François Lavoué, Nicolas L. Celli, and Andrew J. Schaeffer

The enigmatic radial anisotropy of the upper mantle remains difficult to resolve. Recent global models show strong disagreements and suggest different inferences on mantle dynamics and evolution. Here, we present a new radially and azimuthally anisotropic shear-wave velocity model of the upper mantle, LLCS-2026, and validate its key patterns using independent seismic and thermodynamic phase-velocity inversions for tectonic-type-average 1D profiles. LLCS-2026 is computed using waveform fits of 1,630,432 seismograms (1,252,717 vertical; 377,715 transverse components). Automated multimode waveform inversion is used to extract structural information from surface and S waveforms in very broad period ranges, from 11 to 450 s, with most data sampling in the 20–350 s period range. The vertical and transverse component waveforms are jointly inverted for the isotropic average shear-wave velocities, their pi-periodic and pi/2-periodic azimuthal anisotropy, and radial anisotropy. Statistical and manual outlier analysis yields a final dataset of 1,009,038 seismograms (765,302 vertical, 243,736 transverse components) that constrains the final model, which captures complex patterns of seismic isotropic and anisotropic structure within the Earth. In agreement with previously published models, prominent low-velocity anomalies indicative of thin lithosphere and partial melting are observed at 20-150 km depth beneath mid-ocean ridges. At 300-400 km, however, high isotropic-average velocities are present in the vicinity of some of the ridges in the Indian and Atlantic oceans. They suggest drips of cold, lithospheric mantle material, probably related to rapid lithospheric cooling in the complex 3D context of triple junctions and ridge-hotspot systems. Radial anisotropy is positive (Vsh > Vsv) at 100-150 km depth everywhere in the mantle, with cratons showing smaller anisotropy compared to other units. Below 200-250 km depth, radial anisotropy is negative (Vsv > Vsh) nearly everywhere. The depth at which the anisotropy sign changes varies with tectonic region. The anisotropy sign flips at the shallowest depth (~200 km) beneath young oceans and continents and at the greatest depth (~250 km, on average) beneath cratons. Radial anisotropy is also negative in the top 50 km of the oceanic lithosphere. Together with azimuthal anisotropy observations, this indicates a complex pattern of crystallographic preferred orientations created by mantle flow beneath mid-ocean ridges, with an interplay between the alignment of crystals due to the vertical flow below the ridge and the lateral flow away from it. Independent seismic (Civiero et al. 2024) and thermodynamic (Lebedev et al. 2024; Xu et al. 2025) inversions of phase-velocity data confirm and validate the anisotropy-sign-flip observations and inferences.

References

Civiero, C., Lebedev, S., Xu, Y., Bonadio, R. and Lavoué, F., 2024. Toward tectonic‐type and global 1D seismic models of the upper mantle constrained by broadband surface waves. Bulletin of the Seismological Society of America, 114, 1321-1346.

Lebedev, S., Fullea, J., Xu, Y. and Bonadio, R., 2024. Seismic thermography. Bulletin of the Seismological Society of America, 114, 1227-1242.

Xu, Y., Lebedev, S. and Fullea, J., 2025. Average physical structure of cratonic lithosphere, from thermodynamic inversion of global surface-wave data. Mineralogy and Petrology, 1-12.

How to cite: Lebedev, S., Lavoué, F., Celli, N. L., and Schaeffer, A. J.: Radial anisotropy of the upper mantle, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5995, https://doi.org/10.5194/egusphere-egu26-5995, 2026.

EGU26-7464 | Posters on site | GD3.1

AlpRA25: a new radial anisotropy model of the Alps from ambient noise and earthquake surface waves 

Thomas Meier, Henrique Berger Roisenberg, Felix Eckel, Amr El-Sharkawy, Claudio Rosenberg, Lapo Boschi, and Fabio Cammarano

The Alps, together with the Northern Apennines and the Northern Dinarides, represent one of the most complex and best-studied examples of continental collision in the world. Over the years, several active and passive seismic experiments have been deployed in the Alpine region. More recently, the installation of large and dense seismic arrays, such as AlpArray and AdriaArray, has provided unprecedented spatial coverage, enabling the development of increasingly detailed seismic velocity models. However, most existing regional models of the Alps primarily rely on isotropic seismic velocities. Radially anisotropic models, which map the parameter ξ = Vsh²/Vsv², provide complementary information by revealing the preferential orientation of anisotropic minerals and structural fabrics produced by past and ongoing tectonic processes.

In this study, we combine ambient noise and earthquake surface-wave data from more than 3,300 permanent and temporary broadband seismic stations to construct a high-resolution Alpine Radial Anisotropy model (AlpRA25) of the crust and upper mantle. Ambient noise data collected between 2017 and 2019 from approximately 700 seismic stations were used to calculate ~46,000 Rayleigh- and ~40,000 Love-wave dispersion curves. These were merged with ~295,000 Rayleigh- and ~200,000 Love-wave dispersion curves obtained from about 6,000 earthquakes recorded at approximately 3,300 broadband seismic stations between 1990 and 2022, resulting in a total of ~295,000 Rayleigh and ~240,000 Love dispersion curves spanning periods from 3 to 250 s.

These data were inverted for phase-velocity maps using a least-squares algorithm with an average knot spacing of 30 km. An a posteriori outlier analysis discarded 15% of the interstation measurements with the highest residuals, after which the model was recomputed. Local dispersion curves were then extracted at each grid node and evaluated for their frequency-dependent roughness. The Rayleigh and Love local dispersion curves were jointly inverted for 1-D shear-wave velocity structure using a particle swarm optimization algorithm, yielding vertical and horizontal shear-wave velocities (Vsv and Vsh, respectively). The final AlpRA25 model is a high-resolution 3-D model of Vsv, Vsh, and ξ from 5 to 250 km depth, covering the Alps, the Northern Apennines, the Northern Dinarides, and the adjacent foreland and back-arc basins. AlpRA25 provides new constraints on the lithospheric architecture and deformation of the Alpine region, highlighting the role of radial anisotropy in imaging tectonic processes from the crust to the upper mantle.

How to cite: Meier, T., Berger Roisenberg, H., Eckel, F., El-Sharkawy, A., Rosenberg, C., Boschi, L., and Cammarano, F.: AlpRA25: a new radial anisotropy model of the Alps from ambient noise and earthquake surface waves, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7464, https://doi.org/10.5194/egusphere-egu26-7464, 2026.

The Haiyuan Fault, a major strike-slip structure in the northeastern Tibetan Plateau margin, is bounded by the first-order Tibetan Plateau and South China blocks, plus the second-order Ordos and Alxa blocks. Seismic anisotropy serves as a robust proxy for probing deep crustal deformation, geodynamic processes, and subsurface seismic structures. We conducted receiver function analyses on teleseismic data from two dense profiles and five broadband stations across the study area; crustal thickness (42–56 km) and Vp/Vs ratios (1.60–1.88) were quantified by the H-κ domain search algorithm, while common conversion point (CCP) imaging delineated the Moho discontinuity across the Haiyuan Arc Fault Zone. Crustal thickening reflects shortening driven by Tibetan-Eurasian collision, with the Haiyuan tectonic evolution linked to high-temperature/pressure regimes induced by Indo-Asian convergence. CCP images reveal a distinct Moho offset and ambiguous continuity beneath the fault zone, confirming it as a Moho-penetrating transcrustal structure associated with intense crustal extrusion from the plateau interior. We characterized multi-scale crustal anisotropy via shear-wave splitting (SWS) analysis of local earthquake data. SWS parameters exhibit clear zoning controlled by the Haiyuan Fault: fast polarization orientations are NNE–NE north of the fault and WNW–EW south of it. Within ~10 km of the fault, fast orientations align with the fault strike (WNW), indicating the fault’s stress influence range spans dozens of kilometers. Enhanced normalized time-delays near the fault signal stronger anisotropy along this strike-slip belt. Upper crustal anisotropy likely arises from crack-induced fabric, whereas middle-lower crustal anisotropy reflects deformation-controlled fabric. Spatial anisotropy patterns imply the combined effects of stress, faulting, and local tectonics. Notably, SWS results suggest the Haiyuan Fault constitutes the actual crustal boundary of the northeastern Tibetan Plateau, ~200 km north of the previously reported plateau block boundary.

How to cite: Shi, Y. and Gao, Y.: Crustal Deformation of the Haiyuan Fault Zone Inferred from Dense Seismic Array Observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8643, https://doi.org/10.5194/egusphere-egu26-8643, 2026.

EGU26-8791 | Posters on site | GD3.1

Crustal Anisotropy Characteristics in the North China Craton 

Qiong Wang, Yuan Gao, and Geng Liu

    The North China Craton (NCC) exhibits a marked east-west contrast in its present-day tectonic framework. The eastern region  features a thinned lithosphere hosting extensional basins like the Zhangjiakou-Bohai seismic belt and the Shanxi Graben. This area experiences intense crustal deformation and frequent seismicity. Conversely, the western region possesses a thicker lithosphere, greater crustal stability, and weak seismic activity. The central orogenic belt acts as a transitional zone in crust-mantle structure, characterized by dramatic crustal thickness variations, evidence of lithospheric modification, remnants of ancient structures, and is key for studying crust-mantle coupling/decoupling. 
    Crustal anisotropy serves as a crucial indicator for revealing lithospheric deformation. Analysis of seismic wave velocity anisotropy quantitatively constrains crustal stress, assesses fault activity, and infers deep material flow. This provides  essential constraints for seismic hazard assessment and tectonic dynamics research.
    This study utilized local-earthquake data (M>1) from the National Fixed Seismic Network to investigate crustal anisotropy across the NCC using the SAM (Shear-wave splitting Analysis Method) method. The extensive dataset, covering multiple temporal windows of seismic activity, provides strong temporal continuity and spatial coverage for analyzing anisotropy characteristics. Results reveal complex fast-wave polarization directions (FPDs) across the study area. The average FPD (~73°) aligns well with the regional mean maximum horizontal compressive stress (SHmax) direction in the NCC. However, the FPDs also display distinct local features correlating with specific structures, indicating significant local variability in the regional stress field. This manifestation of localized crustal anisotropy characteristics is vital for understanding the region's geodynamic activity. The local stress field variations suggest a heterogeneous crustal stress distribution, likely influenced by multiple geological factors.

How to cite: Wang, Q., Gao, Y., and Liu, G.: Crustal Anisotropy Characteristics in the North China Craton, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8791, https://doi.org/10.5194/egusphere-egu26-8791, 2026.

EGU26-9651 | ECS | Orals | GD3.1

Multi-scale Seismic Anisotropy of the Rotondo Granite: Linking Deformation Fabrics to Wave Propagation 

Emily Hinshaw, Alberto Ceccato, Alba Zappone, Whitney Behr, and Anne Obermann

We investigate the seismic anisotropy of the Rotondo granite (Gotthard Massif, Swiss Alps) by integrating geological and geophysical data from lab to field scale. We compare our modeled anisotropic properties with decameter measurements from boreholes and kilometer-scale regional seismicity data from the Bedretto Underground Laboratory for Geosciences and Geoenergies, demonstrating clear links between deformation fabrics and observed seismic anisotropy across scales. 

Using field- and micro-scale analyses of deformation styles and fabric orientations, we delineate discrete structural domains characterized by varying strain intensities and fabric types, ranging from isotropic granite to fractured zones or proto-mylonitic shear zones. Proto-mylonitic zones exhibit strong phyllosilicate SPO and higher percentage of Vp anisotropy (~8-27%, range is dependent on compositional variations). Fractured zones vary in frequency within the Rotondo massif and also exhibit elevated Vp anisotropy (>7.5%). For each structural domain, we compute effective elastic stiffness tensors (or 'rock recipes') to characterize their intrinsic seismic velocities. We introduce a new approach for combining multiple lithological “rock recipes” that emphasizes collective impact on bulk anisotropy and spatial context, rather than volume-weighted averaging. 

We observe a scale-dependent shift in anisotropic influence, where the control of ductile fabrics (<20 m) is progressively superseded by fractures as the observational scale increases. When these heterogeneous fabrics are aggregated, destructive interference among strongly anisotropic components reduces the bulk anisotropy to ~2.5%, which is below laboratory measured values. We find good agreement between our theoretical results and cross-borehole effective Vp measurements within the Bedretto Lab. We also find qualitative evidence for anisotropy between event relocation models (e.g. Double Difference or NonLinLoc) of background seismicity in the region at the 1-5 kilometer scale. These results demonstrate consistency in seismic anisotropy estimation across methods and scales, and show the utility of geologically-based anisotropy characterization.

How to cite: Hinshaw, E., Ceccato, A., Zappone, A., Behr, W., and Obermann, A.: Multi-scale Seismic Anisotropy of the Rotondo Granite: Linking Deformation Fabrics to Wave Propagation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9651, https://doi.org/10.5194/egusphere-egu26-9651, 2026.

EGU26-10259 | ECS | Orals | GD3.1

Seismic Anisotropy in the Subducting Slab and Mantle Wedge of the Western Hellenic Subduction Zone from Receiver Functions 

Josefine Ziegler, Stéphane Rondenay, and Nicola Piana Agostinetti

The Western Hellenic Subduction Zone is characterized by a transition from oceanic to continental subduction. The change occurs at the Kephalonian transform fault. However, how this transition takes place at depth remains a topic of discussion. This setting thus provides us with an ideal natural laboratory to investigate how differences in subduction regimes affect the structure and dynamics of the system.
To this end, we compute receiver functions across two seismic arrays from the MEDUSA broadband network, one imaging the oceanic subduction and the other imaging the continental subduction. We computed teleseismic receiver functions and performed harmonic decomposition along both lines. We then inverted these results to image the overriding crust, mantle wedge and slab, in terms of their velocity and anisotropic properties. By comparing the seismic properties of the continental and oceanic slabs, we aim to identify key differences in slab structure, seismic anisotropy, dehydration, and metamorphism between the two subduction regimes.
Preliminary results confirm a dipping low velocity zone in both regimes, corresponding to the slab's crust. Its signal is lost below 60 km in the isotropic component but remains visible to greater depths in the anisotropic component. Furthermore, we identify a low velocity layer within the mantle wedge which could resemble the altered LAB of the overriding plate. What sets the two domains apart is the cutoff depth of the isotropic component of the slab – it can be traced 10 km deeper in the South than in the North – and a generally lower anisotropy in the southern mantle wedge.
Until now the LAB has rarely been observed through conventional receiver function analysis or tomography in subduction zones. We therefore suggest that anisotropic inversion may provide unique insight into the structure of the mantle wedge and the subducting slab.

How to cite: Ziegler, J., Rondenay, S., and Piana Agostinetti, N.: Seismic Anisotropy in the Subducting Slab and Mantle Wedge of the Western Hellenic Subduction Zone from Receiver Functions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10259, https://doi.org/10.5194/egusphere-egu26-10259, 2026.

EGU26-10489 | ECS | Posters on site | GD3.1

3-D Anisotropic Structure of the Upper Mantle beneath the Iranian Plateau Using SKS Splitting Intensity Tomography 

Shiva Arvin, Haiqiang Lan, Ling Chen, Zhaoke Ke, Yi Lin, Li Zhao, and Morteza Talebian

The Iranian plateau, characterized by the Arabia-Eurasia continental collision in the Zagros and the Makran oceanic subduction system, presents a unique opportunity to investigate the underlying processes of lithospheric deformation and upper-mantle dynamics. Previous studies of upper mantle seismic anisotropy, mostly using SK(K)S splitting and occasionally direct S waves revealed complex patterns for the fast axes. The observed rotations of fast axis obtained from S and SK(K)S waves along different tectonic setting, the difference in fast directions between S and SK(K)S phases in central Iran, evidence for two-layer anisotropy, and ambiguity regarding the depth origin of observed anisotropy emphasize the need for further studies. These challenges, together with the pronounced tectonic heterogeneity of the Iranian plateau, call for tomographic approaches that allows for the localization of anisotropic structure. In this study, we utilize SKS splitting intensity tomography to elucidate the depth distribution of the anisotropic properties of the upper mantle beneath the Iranian plateau. Our dataset includes teleseismic events with magnitude above 5.5 and epicentral distances between 90 and 130 degrees recorded by 151 permanent (2015-2021) and 296 temporary seismic stations (2003-2021). We employ a three-dimensional full-wave anisotropy tomography method using splitting intensity, which provides enhanced depth resolution compared to traditional shear wave splitting methods. This method utilizes perturbation theory to establish the linear relationship between splitting intensity and anisotropic parameters, including the azimuth of fast axis and anisotropy strength, and incorporates Green's function databases to efficiently compute the sensitivity or Fréchet kernels. Splitting intensity measurements are inverted to construct a three-dimensional model of upper-mantle azimuthally anisotropic structure beneath the study area. Results show clear lateral differences in anisotropic strength and fast-axis orientation specifically between the Zagros and Alborz regions, as well as the adjacent domains. Vertical profiles illustrate depth-dependent heterogeneous anisotropic structures across the lithosphere–asthenosphere boundary into the asthenospheric upper mantle. These variations likely reflect the combined influence of regional tectonic processes, continental collision, lithospheric deformation, and present-day mantle flow patterns beneath the Iranian plateau. Our results highlight the potential of SKS splitting intensity tomography to resolve complex mantle anisotropy and shed new light on the three-dimensional deformation structure of the upper mantle. The observed lateral and depth variations in anisotropy provide new insights into how the relationship between surface tectonics and upper-mantle deformation varies spatially across major tectonic domains such as the Zagros, Makran, Central Iran, and the Alborz.

How to cite: Arvin, S., Lan, H., Chen, L., Ke, Z., Lin, Y., Zhao, L., and Talebian, M.: 3-D Anisotropic Structure of the Upper Mantle beneath the Iranian Plateau Using SKS Splitting Intensity Tomography, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10489, https://doi.org/10.5194/egusphere-egu26-10489, 2026.

EGU26-10589 | ECS | Posters on site | GD3.1

Seismic Anisotropy Beneath the Dinarides: Implications for Adria-Eurasia Convergence 

Katarina Zailac, Silvia Pondrelli, Simone Salimbeni, and Josip Stipčević

Seismic anisotropy can provide important constraints about deformation processes within the lithosphere and underlying asthenosphere, as well as mantle flow patterns in tectonically complex regions. This study presents observations of seismic anisotropy in the upper mantle beneath the Dinarides and adjacent regions based on teleseismic SKS phase recordings from the AdriaArray temporary deployment, complemented by selected stations from the Croatian permanent seismic network and other available stations in the region. The combined datasets provide improved spatial coverage and allow for a more continuous regional assessment of anisotropic structure beneath the Dinarides.

Seismic anisotropy is investigated using a splitting-intensity approach, applied to teleseismic SKS phases. The splitting intensity quantifies the relative amplitude of the transverse component with respect to the radial component and provides a more robust measure of anisotropic effects. From the azimuthal variation of splitting intensity, the splitting parameters, fast-axis orientation and delay time, can be estimated, enabling direct comparison with earlier shear-wave splitting studies.

The inferred anisotropic pattern beneath the southern Dinarides is regionally coherent with fast axes in the direction perpendicular to the strike of the mountain chain. The fast axes in the Internal Dinarides, on the other hand, are generally pointing in the direction parallel to the strike of the mountain chain, which is also supporting previously published results. New and previously unpublished measurements are presented for stations in the northern Dinarides and in the transitional zone between the Dinarides and the Pannonian Basin, providing improved spatial coverage across this geodynamically important boundary.

This study highlights the importance of dense seismic observations and complementary analysis approaches for resolving anisotropic structures in complex orogenic settings. The expanded dataset and inclusion of splitting intensity measurements provide new constraints on upper-mantle deformation beneath the Dinarides and contribute to a more comprehensive understanding of the coupling between lithospheric tectonics and mantle dynamics in the central Mediterranean region. 

How to cite: Zailac, K., Pondrelli, S., Salimbeni, S., and Stipčević, J.: Seismic Anisotropy Beneath the Dinarides: Implications for Adria-Eurasia Convergence, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10589, https://doi.org/10.5194/egusphere-egu26-10589, 2026.

EGU26-11156 | Orals | GD3.1

A review of the sensitivity of seismic wave velocity and attenuation to fracturing 

Nicolas Barbosa, German Rubino, Eva Caspari, and Klaus Holliger

Fractures are ubiquitous throughout the Earth’s upper crust, spanning scales from microscopic cracks to large fault systems. Their hydromechanical behavior plays a critical role in controlling fluid migration in hydrocarbon, geothermal, and groundwater reservoirs, which, in turn, makes fracture detection, characterization, and monitoring an important objective in geoscience and engineering applications. Seismic methods, as indirect and non-invasive tools, have become central to this effort due to their ability to probe fractured media with adequate resolution and depth penetration. This work synthesizes our recent experimental and theoretical advances in the study of seismic characterization of fractured rocks, driven by several key observations. First, most fractured reservoirs exhibit effective seismic anisotropy because fractures often develop preferentially aligned with the local principal stress directions, leading to direction-dependent wave propagation. This anisotropy can be estimated using techniques such as shear-wave splitting, azimuthal velocity variations, and amplitude variations with offset and azimuth. Furthermore, we show that incorporating both fracture-induced and intrinsic background anisotropy, a rather common scenario in fractured environments, into inversion workflows is essential for a robust interpretation. Second, when a seismic wave propagates through a fluid-saturated fractured reservoir, it will be significantly attenuated and dispersed as a result of multiple intrinsic (e.g., inelastic effects due to solid and/or fluid friction effects) and extrinsic (e.g., geometrical spreading) mechanisms. In particular, when a seismic wave propagates through a fluid-saturated porous rock containing fractures, it produces fluid pressure gradients between the more compliant fractures and the stiffer embedding rock as well as between hydraulically connected fractures with different orientations and/or properties. Consequently, fluid flows until the pressure equilibrates, a phenomenon commonly referred to as wave-induced fluid flow (WIFF). This mechanism can alter the effective compliance of the fractures. Such compliance changes can significantly influence velocity and attenuation anisotropy across the seismic frequency range. The dependence of this type of mechanism on the petrophysical properties, fracture-geometry, and distribution makes the analysis of frequency-dependent seismic attributes particularly informative with regard to the hydromechanical properties. [NB2] Third, seismic responses in fractured media are highly sensitive to changes in their stress state, fluid saturation, and geometrical properties, thus, facilitating corresponding monitoring efforts through time-lapse seismic surveys. Finally, highly permeable fractures can often be directly imaged since open fractures with partial surface contacts generally have large mechanical compliance, which, in turn, produces strong scattering of seismic waves. Indeed, there is evidence from full-waveform sonic log data to suggest that the fracture mechanical compliance obtained from P-wave velocity changes and transmission losses correlates with the degree to which fractures are hydraulically open.

How to cite: Barbosa, N., Rubino, G., Caspari, E., and Holliger, K.: A review of the sensitivity of seismic wave velocity and attenuation to fracturing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11156, https://doi.org/10.5194/egusphere-egu26-11156, 2026.

EGU26-12795 | ECS | Posters on site | GD3.1

Crustal Anisotropy Variations Revealed by Local S-wave Splitting in the Source Region of 2023 Kahramanmaraş Earthquakes along the East Anatolian Fault Zone 

Ceyhun Erman, Paola Baccheschi, Seda Yolsal-Çevikbilen, Tuna Eken, and Tuncay Taymaz

The 2023 Kahramanmaraş earthquake doublet (Mw 7.8 and Mw 7.7) produced an extensive rupture along several segments of the East Anatolian Faults (EAF), and triggered intense aftershock activity in southeastern Türkiye. This seismic sequence therefore provides an exceptional dataset to investigate the crustal anisotropy in such a complex tectonic area. In this study, we evaluated the crustal anisotropy in the source region of these catastrophic earthquakes by conducting a detailed local S-wave splitting (SWS) analysis on a relocated earthquake catalogue. We have performed shear-wave splitting measurements over several thousand local-S waveforms recordings of 31 permanent broadband seismic stations operated by AFAD (Turkish Earthquake Data Center) that were extracted using precise relocation of aftershock activity. After a visual quality control procedure for each splitting analysis, a total of 486 high-quality measurements were obtained. The results reveal a highly heterogeneous anisotropic pattern, with fast direction oriented from N80°W to N79°E and mean fast direction for the whole dataset of N16°E, reflecting the lateral variations in the regional stress field along the EAF, the Sürgü-Çardak Fault (SÇF), and the Malatya Fault. A transition between stress-induced and structure-related anisotropy is clearly identified across different segments of the EAF. Stations in close proximity to the EAF exhibit a dominant structure-induced anisotropic signature, characterized by the strict alignment of FPDs parallel to the fault geometry. Overall, the obtained results provide a comprehensive perspective on how the upper crust responds to substantial stress release, thus offering critical insights into the mechanical behaviour of complex fault networks where the regional collisional stress regimes and strike-slip faulting systems converge.

How to cite: Erman, C., Baccheschi, P., Yolsal-Çevikbilen, S., Eken, T., and Taymaz, T.: Crustal Anisotropy Variations Revealed by Local S-wave Splitting in the Source Region of 2023 Kahramanmaraş Earthquakes along the East Anatolian Fault Zone, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12795, https://doi.org/10.5194/egusphere-egu26-12795, 2026.

EGU26-13229 | ECS | Posters on site | GD3.1

Joint body- and surface-wave probabilistic transdimensional tomography of upper mantle seismic anisotropy 

Gianmarco Del Piccolo, Joseph Byrnes, James Gaherty, Brandon VanderBeek, Manuele Faccenda, and Andrea Morelli

Body- and surface-wave seismic data provide complementary sensitivities to the anisotropic elastic structure of the Earth, and the potential constraints of a simultaneous inversion would extend significantly beyond those of the individual phases. However, joint body- and surface-wave anisotropic imaging remains limited, mainly because of the high nonlinearity of the problem and the different inversion methods traditionally adopted for body- and surface-wave phases. Here, we implement a nonlinear transdimensional stochastic solver based on the reversible-jump Markov chain Monte Carlo (RJMCMC) algorithm to simultaneously invert P-, S- and Rayleigh-wave data. By sampling irregularly meshed anisotropic velocity models for the upper mantle, with different mesh configurations and complexities adaptable to the heterogeneous data constraints, we populate an ensemble of variable solutions describing the data within the uncertainties. The method is validated using independent synthetic seismograms simulated with SPECFEM3D Globe in an anisotropic upper mantle plume model. We show how the different sensitivities of the data translate into different constraints on upper mantle seismic structure, and we analyze metrics to quantitatively assess uncertainties in the inferred solutions.

How to cite: Del Piccolo, G., Byrnes, J., Gaherty, J., VanderBeek, B., Faccenda, M., and Morelli, A.: Joint body- and surface-wave probabilistic transdimensional tomography of upper mantle seismic anisotropy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13229, https://doi.org/10.5194/egusphere-egu26-13229, 2026.

Bridgmanite is the most abundant intrinsically-anisotropic constituent of the lower mantle. Its deformation, thus, potentially translates to large-scale anisotropy that would accumulate in high-stress regions, particularly the interaction between subducted materials and the surrounding mantle. While most of the lower mantle is generally considered well-mixed, recent observations suggest structures at mid-mantle depths (800 – 1500 km). Their origin, however, often remains enigmatic. Recent state-of-the-art deformation experiments in bridgmanite at lower-mantle temperatures and pressures reveal a depth-dependent behavior of anisotropy. Coupled with realistic geodynamic models of mantle convection, the large-scale imprint of the depth-dependent fabric reveals a purely deformation-driven seismic discontinuity between 1000 – 1400 km depth that matches observations. The discontinuity appears sharpest in actively deforming regions, and becomes negligible closer to neutral ones. In this work, we investigate its seismic detectability around a subduction zone using three-dimensional global waveform modeling via AxiSEM3D. Given its likely presence across a broad range of frequencies, we assess the suitability of SS precursors for detecting this feature. Enhanced using array seismological methods, results show the presence of SS precursors in the transverse component generated by the anisotropic discontinuity. In addition, a flattened slab geometry produces a shallower SS precursor due to the interface formed between an overlying isotropic slab and an underlying strongly anisotropic (VSH>VSV) layer. We examine the azimuthal dependence of precursor amplitudes and their frequency dependence, with particular emphasis on the microseismic frequency band (~0.05 – 0.25 Hz). In light of these recent findings, we discuss its implications on the nature and origin of mid-mantle discontinuities.

How to cite: Magali, J. K., Yuan, Y., and Thomas, C.: Seismic detectability of a deformation-induced anisotropic discontinuity in the Earth’s lower mantle around a subduction zone using synthetic global modeling of SS precursors, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19103, https://doi.org/10.5194/egusphere-egu26-19103, 2026.

EGU26-1247 | ECS | Posters on site | SM6.4

A 2D joint inversion method for Rayleigh wave phase velocity and attenuation coefficient 

Piao Yang and Youyi Ruan

Seismic attenuation is important to understand the thermal and compositional state of the lithosphere, therefore sheds light on its deformation process. However, measuring the attenuation coefficient of seismic waves is still a challenging task because the phase and amplitude can be affected by both elastic velocity structures and anelastic attenuation, let alone these effects are coupled. Here, we developed a 2D joint inversion T-matrix method for the Rayleigh-wave phase velocity and attenuation coefficient simultaneously. Using a matrix inversion calculation to update the background medium Green functions with scattering series, the scattered wavefield can be fully represented in the frequency domain. First, the T-matrix method takes the coupling of elasticity and attenuation on waveform into consideration by joint inversion. Secondly, by calculating the anelastic scattering effects, 2D distribution can be obtained even for weak attenuation, which is a step towards 3D Q structure. Without time domain wave propagation simulations, the method is affordable in regional problems. Therefore, the method can be used to invert 2D Rayleigh wave phase velocity and attenuation coefficients.

How to cite: Yang, P. and Ruan, Y.: A 2D joint inversion method for Rayleigh wave phase velocity and attenuation coefficient, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1247, https://doi.org/10.5194/egusphere-egu26-1247, 2026.

Characterizing high-frequency (~10 Hz) seismic wave propagation is essential for understanding strong ground motions and improving seismic hazard assessment. High-frequency components are strongly influenced not only by source processes but also by small-scale heterogeneity along the propagation path. In the crust, vertical layering coexists with lateral heterogeneity, which plays a key role in controlling the propagation and attenuation of seismic waves. During propagation, seismic energy is reduced by intrinsic attenuation, in which energy is dissipated into heat and acoustic energy, and by scattering due to heterogeneity, which can produce apparent attenuation or amplification. In this study, we analyze S-wave coda from the 2016 Gyeongju earthquake using Multiple Lapse Time Window Analysis (MLTWA) to estimate the intrinsic (Qi), scattering (Qs), and total (Qt) quality factors in discrete frequency bands. Over the central frequency range of 1.5–22 Hz, the inferred Qs values range from approximately 398 to 4399, Qi from 185 to 1390, and Qt from 120 to 1041, revealing a pronounced frequency dependence of attenuation. The observed Qs–frequency relationship is then interpreted using a von Kármán autocorrelation model, yielding crustal heterogeneity parameters ε = 0.048, κ = 0.32, and a = 8.0 km. These parameters reproduce the empirical Qs curve and are used to generate random heterogeneous media for numerical simulations of high-frequency wave propagation. By integrating observation-based heterogenous crustal modeling, this study quantitatively constrains the influence of crustal heterogeneity on high-frequency seismic wave propagation and provides a physical basis for refining strong ground motion prediction models and improving the reliability of seismic hazard assessments.

How to cite: Lee, S., Cho, C. S., and Song, S. G.: High-Frequency Seismic Wave Simulations in Qs-Constrained von Kármán Random Media for the 2016 Gyeongju Earthquake, South Korea, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2494, https://doi.org/10.5194/egusphere-egu26-2494, 2026.

EGU26-2933 | Orals | SM6.4

Integrating Seismic Anisotropy, Attenuation, and Machine Learning for Advanced Subsurface Characterization 

Fateh Bouchaala, Jun Matsushima, and Guibin Zhao

Seismic anisotropy and attenuation, often quantified by the inverse of the quality factor (), are powerful, but often underexploited, indicators of fracture architecture, fluid content, and small-scale heterogeneity in the subsurface. At the same time, machine-learning (ML) methods offer flexible, data-driven mappings between seismic attributes and subsurface properties yet are not often designed to exploit seismic anisotropy and attenuation. In this contribution, an integrated workflow that combines laboratory measurements, borehole and VSP data, and surface seismic attributes with ML modelling to achieve advanced subsurface characterization in fractured carbonate systems.

Seismic waveforms collected in Abu Dhabi in the United Arab Emirates (UAE), were recorded at wide frequency range from Hertz to MHz, in the field and laboratory. The lithology of Abu Dhabi subsurface is dominated by carbonates, which are known by their high heterogeneity and multiple fracturing systems. To address the complexity caused by lithology, new methods and processing workflows have been developed and applied on the data. This includes new methods for calculating seismic attenuation from surface seismic, vertical seismic profiling (VSP), and sonic data, allowing an estimate of attenuation magnitude and its anisotropy, in addition to separating between scattering and intrinsic attenuation.

The study includes a suite of field and laboratory studies that quantify azimuthal P-wave attenuation, separate intrinsic and scattering contributions, and relate these to fracture systems and tar-mat occurrence in Abu Dhabi carbonate subsurface. These include multi-offset azimuthal VSP analyses that recover fracture strike and discriminate between open and cemented fractures using attenuation anisotropy, detailed attenuation-mode separation from VSP and sonic data, AVAz-based fracture characterization from 3D surface seismic, and ultrasonic measurements that document the sensitivity of  to petrophysical properties and saturation in carbonate core plugs. Building on this physical understanding, we extend recent work on ML-based prediction of Thomsen’s parameters from synthetic and VSP data to explicitly incorporate multi-scale attenuation attributes. Training data is generated by finite-difference modeling in anisotropic, fractured carbonate media constrained by well logs, FMI, and core information from an offshore Abu Dhabi oilfield. Input features include azimuthally dependent amplitudes of direct and reflected waves, frequency- and traveltime–derived attributes. We benchmark several ML regressors (support vector regression, extreme gradient boosting, multilayer perceptrons, and 1D convolutional neural networks) and use explainable AI tools to rank the relative importance of attenuation- versus kinematics-based features.

This study demonstrates that jointly exploiting anisotropy, attenuation, and ML substantially improves the interpretability and resolution of fracture and fluid systems in complex carbonate media. The proposed workflow is generic and can be transferred to other fractured and heterogeneous settings, offering a practical route to physics-aware, data-driven seismic characterization for reservoir development and monitoring. 

How to cite: Bouchaala, F., Matsushima, J., and Zhao, G.: Integrating Seismic Anisotropy, Attenuation, and Machine Learning for Advanced Subsurface Characterization, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2933, https://doi.org/10.5194/egusphere-egu26-2933, 2026.

EGU26-3654 | Posters on site | SM6.4

A high-resolution broadband crustal Lg attenuation model beneath Colombia and its implication for triple-junction tectonics 

Lian-Feng Zhao, Zhen Liu, Xiao-Bi Xie, Carlos A. Vargas, Baofeng Tian, and Zhen-Xing Yao

The existence of a typical triple junction in Colombia is crucial for understanding plate convergence and coupling among the South American Plate, the subducting Nazca Plate, and the Caribbean Plate. However, locating this triple junction is challenging due to complex geodynamic evolution and uncertainty in the slab boundaries. Here, we developed a high-resolution Lg-wave attenuation model for Colombia and surrounding areas to constrain crustal magmatic activity, link deep processes with surface volcanism, and identify potential slab boundaries. The area encompassing Central America, western Colombia, and Ecuador exhibits strong Lg attenuation and a concentration of volcanoes, indicating thermal anomalies in the crust. In line with the velocity structure, volcanism, seismicity, and isotopic dating, the thermal anomalies associated with the subducting Nazca and Caribbean slabs suggest the presence of three subducting slabs beneath the South American Plate, with a triple junction located at approximately 7.5°N, 77°W. This research was supported by the National Natural Science Foundation of China (42430306).

How to cite: Zhao, L.-F., Liu, Z., Xie, X.-B., Vargas, C. A., Tian, B., and Yao, Z.-X.: A high-resolution broadband crustal Lg attenuation model beneath Colombia and its implication for triple-junction tectonics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3654, https://doi.org/10.5194/egusphere-egu26-3654, 2026.

Anelasticity is an intrinsic property of Earth’s interior and it is closely associated with temperature, partial melt, and water content. To date, the development of seismic attenuation models has lagged behind that of velocity models, due to the difficulty in distinguishing attenuation effects from velocity heterogeneities in waveforms, as well as inconsistencies across inversion methods and their resulting attenuation structures. To address these challenges, we recently developed a novel anelastic scattering-integral-based full waveform inversion (FWI) method. Its effectiveness has been verified through numerical experiments using the Northwestern United States region as a realistic case study. Specially, the method can accurately solve 3D anelastic wave equation even in the presence of strong attenuation and computes full anelastic sensitivity kernels incorporating both effects of physical dispersion and dissipation. As an application, we utilize abundant seismic waveform data from the China National Seismic Network to establish, for the first time, a high-resolution 3D anelastic structure model of the lithosphere and asthenosphere in the eastern Tibetan Plateau. Waveform comparisons and checkerboard tests verify the reliability of the inverted model, which achieves a maximum horizontal resolution of 0.6°×0.6°and a maximum vertical resolution of 25 km. This highly accurate anelastic model provides important structural constraints for understanding the deep processes of material extrusion at the eastern margin of the Tibetan Plateau.

This work is supported by the National Natural Science Foundation of China (42204056).

How to cite: Wang, N.: 3D anelastic full waveform inversion and its application, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4131, https://doi.org/10.5194/egusphere-egu26-4131, 2026.

EGU26-4344 | Posters on site | SM6.4

Probing Mantle Deformation beneath the Southern Granulite Terrain Using Seismic Attenuation Anisotropy 

Ritima Das, Faris Hamza, and Utpal Saikia

The Southern Granulite Terrain (SGT) in peninsular India is a high-grade metamorphic region formed by intricate Precambrian tectonic processes, serves as a natural laboratory for examining the seismic properties of solid continental lithosphere. Attenuation anisotropy shows how seismic energy loss changes with direction, giving extra information beyond just how fast seismic waves move through rock. It is particularly good at showing processes like grain-boundary relaxation, dislocation creep, and fluid assisted deformation. We have measured the shear-wave splitting parameters (, ) and attenuation anisotropy (, ) for the SKS phases recorded at 13 stations spread over the SGT using the second eigenvalue minimisation method and the instantaneous frequency matching technique, respectively. The attenuation anisotropy parameters for each station, obtained through a weighted-stacking process, vary from 0.1s to 0.85s for differential attenuation () with an average of ~0.36s and -82° to 88° for fast polarisation direction (), with the apparent fast wave () attenuating more, indicating the presence of fluid-filled fractures. Removing the attenuation effects, the station-averaged delay time () lies between 0.73s and 1.27s, with an average of ~0.99s, and fast polarisation direction () lies between -87° and 58°. We further analysed the backazimuthal dependence of the splitting parameters. The melt inclusions and the anisotropic layers beneath each station are characterised using the squirt flow model. The fractures are striking at an angle between ~49° and ~306°, and dipping at an angle between ~36° and 50°. The anisotropic layer thickness varies from 33 km to 115 km beneath the stations. Variations in attenuation anisotropy across major shear zones, like the Palghat–Cauvery and Achankovil sutures, offer important information about reactivated shear deformation, fossil lithospheric fabrics, and potential asthenospheric contributions in the SGT. This information helps to clarify the tectonothermal evolution of this ancient crustal block.

How to cite: Das, R., Hamza, F., and Saikia, U.: Probing Mantle Deformation beneath the Southern Granulite Terrain Using Seismic Attenuation Anisotropy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4344, https://doi.org/10.5194/egusphere-egu26-4344, 2026.

EGU26-4670 | ECS | Orals | SM6.4

Crustal Lg and upper mantle Pn attenuation structure beneath the Yangtze craton and its implications for the ancient cratonic nucleus 

Lin Shen, Lian-Feng Zhao, Xu Chang, Xiao-Bi Xie, and Zhen-Xing Yao

Cratons are traditionally considered to be long-lived and stable owing to their great thickness and rigid lithospheric roots. However, increasing evidence suggests that some cratons have experienced significant lithospheric thinning and destruction. The Sichuan basin, a cratonic basin within the Yangtze Craton, is widely regarded as the cratonic nucleus owing to its long-term tectonic stability and continuous sedimentary subsidence. However, the oldest Archean basement of the Yangtze Craton, represented by the Kongling Complex, is mainly exposed in the eastern Sichuan Basin, raising the question of the spatial location of the ancient nucleus for the Yangtze Craton. Since the Mesozoic, the Yangtze Craton has been affected by the combined influences of Paleo-Pacific subduction and Cenozoic eastward extrusion of the Tibetan Plateau, and the preservation and spatial distribution of its deep lithospheric root remain poorly constrained by geophysical observations. Here, we constructed a high-resolution crustal-upper mantle attenuation model using regional Pn and Lg phases to constrain the coupling/decoupling characteristics between crust and upper mantle beneath the Yangtze Craton. The weak crustal Lg attenuation in the Sichuan Basin does not correspond to the weak Pn attenuation in the upper mantle, indicating that the lithospheric root may mechanically migrate to the eastern Sichuan Basin. The phenomenon is likely associated with the Cenozoic eastward extrusion of the Tibetan Plateau, yet the eastern Yangtze Craton appears to have undergone overall lithospheric thinning and destruction related to Mesozoic Paleo-Pacific subduction. This study was supported by the National Natural Science Foundation of China (42474084) and Deep Earth Probe and Mineral Resources Exploration-National Science and Technology Major Project (2025ZD1005302).

How to cite: Shen, L., Zhao, L.-F., Chang, X., Xie, X.-B., and Yao, Z.-X.: Crustal Lg and upper mantle Pn attenuation structure beneath the Yangtze craton and its implications for the ancient cratonic nucleus, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4670, https://doi.org/10.5194/egusphere-egu26-4670, 2026.

EGU26-4722 | Posters on site | SM6.4

Rayleigh-wave attenuation in the southern Korean Peninsula from Helmholtz tomography 

Seungwoo Park and Sung-Joon Chang

Seismic attenuation offers insights into subsurface material properties, which are independent of the velocity information obtained from seismic tomography. Because seismic‐wave amplitude attenuation is sensitive to several factors such as temperature, mineral grain size, partial melt, and compositional variations, quantitative attenuation analysis provides additional constraints on the thermal and rheological state of the Earth’s interior. However, compared to seismic imaging studies, attenuation characteristics of the subsurface beneath the southern Korean Peninsula remain poorly constrained. In this study, we analyze seismic waveforms recorded at approximately 40 broadband seismic stations deployed across the southern Korean Peninsula between 2009 and 2012, and derive preliminary Rayleigh-wave attenuation estimates over the period range of 20–120 s. The results show generally low attenuation at short periods (20–30 s), which are primarily sensitive to the crust and uppermost mantle, whereas relatively high attenuation is observed at longer periods (80–120 s), corresponding to asthenospheric depths. These patterns likely reflect increasing temperature and rheological heterogeneity in the upper mantle. Future work will expand station coverage and invert the attenuation measurements to construct a detailed depth‐dependent attenuation model beneath the southern Korean Peninsula.

How to cite: Park, S. and Chang, S.-J.: Rayleigh-wave attenuation in the southern Korean Peninsula from Helmholtz tomography, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4722, https://doi.org/10.5194/egusphere-egu26-4722, 2026.

EGU26-5110 | ECS | Posters on site | SM6.4

Multi-parameter seismic attenuation tomography of the Calabrian crust (Italy) using MuRAT3D 

Gaia Caporale, Mario La Rocca, Rita de Nardis, and Luca De Siena

Abstract

Seismic attenuation, controlled by scattering and intrinsic absorption processes, represents a fundamental property for investigating crustal heterogeneity, fracturing, and fluid distribution. Here we present results from 3D attenuation tomography in the Calabrian Arc (Southern Italy), based on a relocated local-earthquake dataset analyzed within the MuRAT3D framework (De Siena et al. 2014). The study relies on a dedicated dataset of ~490 local earthquakes recorded between 2016 and 2024 by integrating local and national seismic networks. Event selection was designed to ensure homogeneous spatial and depth coverage while limiting clustering effects. P- and S-wave arrivals were manually picked, and earthquakes were relocated using a combined deterministic–probabilistic approach, producing a robust dataset optimized for attenuation analysis (Schweitzer, 2001; Chiappetta and La Rocca, 2024).

MuRAT3D enables a multi-parameter characterization of seismic energy loss by exploiting different portions of the seismic waveform. Scattering is investigated through Peak Delay (PD) derived from envelope broadening, while total and intrinsic attenuation are described by the quality factors Q and Qc. Analyses were carried out at discrete frequencies (1.5, 3, 6, 12, and 18 Hz), showing that only specific frequency bands yield stable and physically consistent attenuation parameters, reflecting the validity limits of the underlying assumptions and different seismic wave propagation regimes. The resulting 3D attenuation images display coherent, laterally variable patterns, with strong contrasts between continental and offshore domains and localized anomalies related to pronounced crustal heterogeneities and possible interactions with deep structures.Ongoing analyses aim to further refine attenuation patterns and their geological interpretation.

How to cite: Caporale, G., La Rocca, M., de Nardis, R., and De Siena, L.: Multi-parameter seismic attenuation tomography of the Calabrian crust (Italy) using MuRAT3D, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5110, https://doi.org/10.5194/egusphere-egu26-5110, 2026.

EGU26-5341 | ECS | Orals | SM6.4

Pn-wave attenuation tomography in Anatolia and its implications for slab break-off, mantle upwelling, and plateau uplift 

Qing-Yang Cheng, Lian-Feng Zhao, Tuna Eken, Xiao-Bi Xie, Hong-Yi Li, and Zhen-Xing Yao

Within the collision zone between the Arabian and Eurasian plates, the Anatolian Plateau represents an early stage in the closure of the Neo-Tethys Ocean (Teknik et al., 2025). The uplift mechanism of the Anatolian Plateau remains debated, as the primary geodynamic drivers likely vary regionally. While upper-crustal shortening dominates the northern margin of Central Anatolia, slab break-off and mantle upwelling are key along the southern and interior margins (Şengör et al., 2008; Yildirim et al., 2011). These processes are not isolated but may be geodynamically linked through subsequent shifts in plate motion and mantle flow following slab break-off. The Pn wave is a seismic phase that propagates primarily within the uppermost mantle. Its attenuation characteristics serve as a proxy for physical properties such as temperature, pressure, and water content in this region. Therefore, high-resolution attenuation tomography of the uppermost mantle using Pn waves can provide key constraints on the tectonic evolution of the Anatolian Plateau. 

In this study, we collected 23,830 seismic waveform data from 853 events recorded by 717 seismic stations between July 1996 and August 2025. Using a joint inversion method (Zhao et al., 2015), we constructed a broadband (0.05 - 20.0 Hz) high-resolution (1.0  1.0) Pn-wave attenuation model for the Anatolian Plateau. A prominent high-Q region observed in the southwestern part of the study area represents the Aegean Slab while a localized high-Q zone surrounded by low-Q anomalies (at approximately 36°E, 39°N) correlates with volcanism in the Central Anatolian Plateau. This work was supported by the National Natural Science Foundation of China (No. 42430306).

How to cite: Cheng, Q.-Y., Zhao, L.-F., Eken, T., Xie, X.-B., Li, H.-Y., and Yao, Z.-X.: Pn-wave attenuation tomography in Anatolia and its implications for slab break-off, mantle upwelling, and plateau uplift, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5341, https://doi.org/10.5194/egusphere-egu26-5341, 2026.

Seismic attenuation provides key constraints on the thermo-mechanical state and small-scale heterogeneity of the crust, but high-frequency observations are strongly affected by the coupling between intrinsic attenuation (Qi) and scattering attenuation (Qsc). This coupling hampers conventional attenuation inversions, particularly in tectonically complex regions such as the eastern margin of the Tibetan Plateau. High-frequency seismic coda wave envelopes provide critical insights into the influence of attenuation structures on energy evolution and serve as an essential data source for scattering studies.  In this study, we combine unsupervised machine learning and physics-based envelope modeling to investigate crustal intrinsic and scattering attenuation across the Longmenshan Fault Zone and adjacent regions. We first apply a Conditional Variational Autoencoder (CVAE) to tens of thousands of high-frequency (2–4 Hz) P- and S-wave envelopes, including their coda, recorded by a regional seismic array. By conditioning on source–receiver distance, the CVAE suppresses geometric effects and extracts latent variables that characterize lateral and vertical variations in envelope shape. Two latent variables are sufficient to describe the dominant envelope features: the first is primarily associated with variations in P-to-S energy ratios and correlates with intrinsic attenuation, while the second reflects changes in envelope width and peak timing, consistent with scattering strength. The spatial distribution of the intrinsic-attenuation-related latent variable reveals a clear contrast between the Tibetan Plateau and the Sichuan Basin, whereas scattering-related variations are mainly controlled by local small-scale heterogeneity and show no systematic dependence on large-scale tectonic units. Guided by these results, we further perform three-dimensional high-frequency envelope modeling using radiative transport theory on ~61,000 three-component seismograms. We constructed two-layer models of intrinsic attenuation and small-scale scattering structures for the crust of Sichuan Basin and Tibetan Plateau regions, respectively. The sedimentary layer of the Sichuan Basin displays strong scattering and intrinsic attenuation, suggesting a porous, potentially fluid-rich structure, which aligns with the presence of abundant oil and gas resources. The relatively weak scattering and intrinsic attenuation in the Sichuan Basin's crust indicate its nature as an ancient, stable geological block. The lower crust of the Tibetan Plateau shows stronger intrinsic attenuation than the upper crust but significantly weaker scattering, suggesting the presence of a high-temperature, viscous flow structure in the region. The upper crust of the Tibetan Plateau exhibits significantly stronger scattering and intrinsic attenuation compared to that of the Sichuan Basin, reflecting the extensively faulted and fractured structure due to ongoing tectonic collisions.

How to cite: Zhang, B., Li, J., Ni, S., and Zhang, H.: Crustal Scattering and Intrinsic Attenuation Across the Eastern Margin of the Tibetan Plateau Revealed by High-Frequency Coda Waves, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6112, https://doi.org/10.5194/egusphere-egu26-6112, 2026.

EGU26-6591 | ECS | Orals | SM6.4

Spatiotemporal monitoring of soil moisture dynamics from Rayleigh-wave attenuation: A controlled field experiment 

Xinyu Liu, Binbin Mi, Jianghai Xia, Jianbo Guan, Jie Zhou, and Haoyuan Sun

Seismic attenuation provides a highly sensitive constraint on fluid-driven processes in the shallow subsurface. These attenuation-derived spatiotemporal insights complement conventional seismic velocity monitoring and can be used for environmental monitoring and engineered subsurface infrastructure management. In this study, we implemented time-lapse Rayleigh-wave attenuation measurements during controlled shallow water injections to quantify the coupled evolution of seismic attenuation and pore-fluid infiltration. The monitoring experiment was conducted over a 14-day period at a localized test site where two vertical wells were hydraulically connected by a permeable pipeline. The frequency-dependent Rayleigh-wave attenuation coefficients are estimated from spectral-ratio slope fitting of multichannel active-source surface-wave records. These measurements are subsequently combined with phase velocities and S- and P-wave velocities to invert for depth-dependent energy dissipation factors  and  within a layered medium. The resulting attenuation variations are interpreted as proxies for changes in fluid saturation and hydrological properties in the shallow subsurface. The attenuation images clearly delineate the boundary between the pipeline and the surrounding medium and exhibit pronounced temporal variations driven by injection-induced fluid migration. Daily time-lapse variations of attenuation over the 14-day experiment reveal frequency-dependent responses to the intermittent injection schedule, with peak values near the period of maximum injection. These patterns reflect the migration and redistribution of pore fluids within the near-surface formation. The inverted Q images further identify localized low-Q zones around the pipeline and the two wells, indicating enhanced energy dissipation associated with fluid accumulation and increasing saturation. This study establishes a powerful framework for monitoring fluid migration and its physical impacts from time-lapse seismic attenuation. Our results highlight the importance of attenuation-based imaging for advancing high-resolution characterization of near-surface hydrological and engineered subsurface environments.

How to cite: Liu, X., Mi, B., Xia, J., Guan, J., Zhou, J., and Sun, H.: Spatiotemporal monitoring of soil moisture dynamics from Rayleigh-wave attenuation: A controlled field experiment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6591, https://doi.org/10.5194/egusphere-egu26-6591, 2026.

We estimated shear-wave splitting parameters and splitting intensity using core-refracted phases (SKS and SKKS) recorded at 90 digital broadband seismic stations across the South Indian Shield, encompassing the Western Dharwar Craton (WDC), Eastern Dharwar Craton (EDC), and Southern Granulite Terrain (SGT). Observed delay times range from 0.4 to 1.5 s, with a mean of ~0.9 s, while fast polarization directions vary from NW to NE–NNE. Although delay times show no significant variation among the three tectonic domains, fast polarization directions exhibit pronounced spatial differences. The EDC is characterized predominantly by NE–NNE orientations, the WDC by N–S to NW directions, and the SGT by a mixed pattern ranging from NW to NE. The splitting intensity varies smoothly across the region, with values ranging from 0.8 to 1.0. These observations suggest that seismic anisotropy beneath the South Indian Shield reflects a complex interplay between the Archean lithospheric architecture and subsequent domain-specific deformation driven by deep Earth processes.

How to cite: Saikia, U., Shameer, S., and Das, R.: Seismic Anisotropy and Splitting Intensity Beneath the South Indian Shield: Evidence for Archean Lithospheric Fabric and Post-Archean Deformation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6793, https://doi.org/10.5194/egusphere-egu26-6793, 2026.

EGU26-6910 | Posters on site | SM6.4

A spectral-ratio-constrained joint inversion of source parameters and attenuation 

Xu Chang, Lin Shen, and Lian-Feng Zhao

Strong trade-offs between earthquake source and attenuation term remain a major challenge in source parameters inversion and attenuation structure. Spectral ratio methods alleviate this problem by using nearby small earthquakes with highly correlated waveforms as empirical Green’s functions (EGF), thereby reducing path and site effects and enabling robust relative estimation of source parameters, particularly corner frequency. However, limited signal-to-noise ratios and spikes at high frequencies significantly affect the estimation of corner frequency. In addition, different choices of EGF may further increase the uncertainty in corner frequency estimations. To reduce the effects of high-frequency spectral instability and EGF selection on spectral ratios, we first perform single-spectrum fitting to obtain physically constrained and smoothed amplitude spectra. These fitted spectra are then used to construct spectral ratios, from which corner frequencies can be robustly estimated. The source parameters constrained by the spectral ratio analysis are then incorporated as prior information, with the introduction of controlled perturbations, a joint inversion of the source parameters (M0 and fc) and the attenuation factor t* is carried out using single spectra fitting. We applied this method to earthquakes that occurred in the southern Sichuan Basin. We applied this method to 257 earthquakes with magnitudes ≥1.5 recorded in the Weiyuan area of the southern Sichuan Basin, China, between November 2015 and November 2016. Seismic moments and corner frequencies are obtained through the combined use of spectral ratio analysis and single spectral fitting, from which stress drops are estimated assuming a circular crack model. The resulting t* measurements are subsequently used to invert for the regional attenuation structure, providing an independent evaluation for the robustness of the inferred source parameters. This study was supported by the National Natural Science Foundation of China (42474084).

How to cite: Chang, X., Shen, L., and Zhao, L.-F.: A spectral-ratio-constrained joint inversion of source parameters and attenuation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6910, https://doi.org/10.5194/egusphere-egu26-6910, 2026.

EGU26-8977 | ECS | Posters on site | SM6.4

Quantifying attenuation and scattering in skull-like phantoms using the spectral element method 

Isha Lohan, Patrick Marty, and Andreas Fichtner

In both geophysics and medical physics, the propagation of seismic waves through highly complex, heterogeneous viscoacoustic-viscoelastic media follows the same physical principles. The attenuation of seismic waves in the Earth's heterogeneous interior is identical to the way ultrasound waves behave when passing through the human skull or bones (transcranial ultrasound).
In this work, we utilize the core concepts of wave physics and spectral element method (SEM), a well-known numerical simulation technique within geophysics that is used to study the scattering and attenuation caused by the skull during transcranial ultrasound. In the Earth, P-waves can convert to S-waves at interfaces; similarly, at the interface of the skull, ultrasound undergo mode conversions, and also generates Lamb waves, which further complicates the energy transmission. Despite the massive difference in physical scale, both medical ultrasound and geophysics involve a similar number of wavelengths between the source and receiver.

The interface between the skull and soft brain tissue creates a high impedance contrast causing most of the energy to reflect and only a small amount of energy is transmitted through skull.
3D numerical phantoms replicating skull-like properties with varying thicknesses were constructed. SEM, a high-order numerical modeling technique, is used for full waveform modeling of both elastic-acoustic and viscoacoustic-viscoelastic waves through heterogeneous media. A conformal hexahedral mesh is implemented to precisely resolve the irregular geometry of the bone. This ensures that the simulated reflections and refractions are physically accurate and thereby avoid numerical staircasing artifacts. 

The difference in the amplitude and waveform propagation is studied between the acoustic-elastic and viscoacoustic-viscoelastic mediums. Elastic modeling assumes energy is conserved, while viscoelastic modeling incorporates the quality factor (Q) to simulate intrinsic attenuation. 
Amplitude decay measures the difference between the peak pressure value of the transmitted waves. Amplitude decay and difference between wavefields are analyzed to quantify how the heterogeneous internal structure affects the wavefront, and also demonstrating that SEM, a proven geophysical method, effectively simulates and quantifies medical ultrasound wave propagation.

How to cite: Lohan, I., Marty, P., and Fichtner, A.: Quantifying attenuation and scattering in skull-like phantoms using the spectral element method, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8977, https://doi.org/10.5194/egusphere-egu26-8977, 2026.

EGU26-9760 | ECS | Orals | SM6.4

Ambient Noise Tomography Reveals Heterogeneous Structure of the Igneous Rocks in Hong Kong’s Upper Crust 

Zhanwen Li, Xi Wang, Xin Liu, Hongfeng Yang, and Guochun Zhao

Hong Kong, one of the most densely populated financial centers in the world, has received limited attention in subsurface structure imaging due to its tectonic quiescence. However, it sits atop the core of the Lianhuashan Fault Zone and was a center of multiple super volcanic eruptions during Yanshanian movement. The complex fault systems and widespread geothermal resources in adjacent region are legacies of these intense tectonic events. We deployed a temporary array of 13 portable seismic nodal sensors covering Hong Kong core area and recorded 21-day seismic data. Using ambient noise adjoint tomography, we imaged the upper 8 km of the crust at high resolution. Significant fault-controlled heterogeneity revealed indicates both geothermal potential and seismic hazard. A deep-seated fault beneath Lantau Island experienced intense fault dilation and volcanic activity as it served as a main magma conduit during Mesozoic. It left behind fractured felsic rocks (low velocity) and rigid mafic intrusions (high velocity), forming a potential seismogenic structure. Pronounced low-velocity anomaly beneath Tai Mo Shan may reflect geothermal activity. Combined with pervasive fracturing and abundant precipitation in Hong Kong, this suggests the presence of an uplift-driven convective geothermal system in the region.

How to cite: Li, Z., Wang, X., Liu, X., Yang, H., and Zhao, G.: Ambient Noise Tomography Reveals Heterogeneous Structure of the Igneous Rocks in Hong Kong’s Upper Crust, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9760, https://doi.org/10.5194/egusphere-egu26-9760, 2026.

EGU26-10547 | ECS | Posters on site | SM6.4

Lg Wave Attenuation across the Indo-Eurasian Collision Zone 

Shirish Bose, Chandrani Singh, and Arun Singh

The collision between the Indian and Eurasian plates has resulted in one of the most tectonically active zones in the world. To characterize the crustal structure and thermal properties of the region, we present a high resolution Lg wave attenuation model along with Lg wave propagation efficiency map for the Indian Shield, the Himalayas, and the Tibetan Plateau and neighbouring areas. Using a dataset comprising more than 1,800 regional earthquakes recorded by 795 broadband seismic stations, we inverted spectral amplitudes using the least squares orthogonal factorization (LSQR) method to map the lateral variation of the Lg wave quality factor (QLg ) and its frequency dependence (η). The resulting tomographic images reveal a sharp contrast in crustal attenuation across the collision zone. The Indian Shield exhibits significant tectonic stability and low attenuation (high QLg ) along with high Lg wave propagation efficiency, consistent with the transmission of seismic energy through a rigid cratonic lithosphere. Conversely, the Tibetan Plateau is dominated by widespread high attenuation (low QLg ) and significantly reduced Lg wave propagation efficiency, with the lowest values observed beneath the Qiangtang and Songpan-Ganzi terranes. The variation in the η parameter highlights the distinction between intrinsic and scattering attenuation, correlating strongly with regional heat flow variations. We observe a clear spatial correlation between low QLg anomalies and the presence of partial melt or aqueous fluids within the Tibetan crust. These results provide new insights into the geophysical understanding of the collision zone and the geometry of the crustal structure.

How to cite: Bose, S., Singh, C., and Singh, A.: Lg Wave Attenuation across the Indo-Eurasian Collision Zone, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10547, https://doi.org/10.5194/egusphere-egu26-10547, 2026.

EGU26-12286 | ECS | Posters on site | SM6.4

New Insight into the Indo-Burma Subduction Zone: Implications from Seismic Attenuation Tomography in Central Myanmar 

Yilin Feng, Yinshuang Ai, Zhuoran Zhang, Yumei He, Mingming Jiang, S. Shawn Wei, Chit Thet Mon, Myo Thant, and Kyaing Sein

Myanmar is located at the southeastern margin of the collision zone between the Indian and Eurasian plates, occupying a key position in the Eastern Himalayan Syntaxis. It serves as a natural laboratory for studying oblique subduction, accretionary orogeny, and crust-mantle dynamics. However, the complex crust-mantle kinematic decoupling mechanism in this region, as well as the control of deep slab geometry on magmatic thermal evolution, remain subjects of debate. Since seismic attenuation is highly sensitive to temperature, partial melting, and fluid content, conducting high-resolution attenuation tomography is crucial for revealing the deep physical state of materials and geodynamic processes in this area. In this study, we performed high-resolution 3-D P-wave attenuation tomography of the Myanmar Orogen using seismic data recorded by 70 stations from the China-Myanmar Geophysical Survey in the Myanmar Orogen (CMGSMO I) between June 2016 and February 2018. We utilized 2,313 seismic events obtained from a deep-learning-based catalog and extracted 14,273 high-quality P-wave t* measurements. By employing the trans-dimensional Bayesian Markov Chain Monte Carlo (MCMC) method, we constructed a high-precision 3-D attenuation model of the study region. The inversion results reveal two significant high-attenuation anomalies: a shallow high-attenuation zone beneath the Indo-Burma Ranges (IBR) at depths of 0–40 km, and a deep high-attenuation anomaly beneath the Central Basin at depths of 80–120 km. The shallow high-attenuation zone coincides well with low-velocity structures; we attribute this to high porosity and fluid saturation within the accretionary wedge sediments, as well as fluid overpressure and rheological weakening caused by deep metamorphic dehydration. This rheologically weak layer likely acts as a lower crustal detachment, facilitating kinematic decoupling between the upper crust and the underlying lithosphere. The deep high-attenuation anomaly reflects asthenospheric upwelling triggered by a "slab window" resulting from the tearing of the Indian Plate. The injection of high-temperature material into the mantle wedge induces partial melting and significantly enhances seismic wave attenuation.

How to cite: Feng, Y., Ai, Y., Zhang, Z., He, Y., Jiang, M., Wei, S. S., Mon, C. T., Thant, M., and Sein, K.: New Insight into the Indo-Burma Subduction Zone: Implications from Seismic Attenuation Tomography in Central Myanmar, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12286, https://doi.org/10.5194/egusphere-egu26-12286, 2026.

EGU26-13919 | ECS | Posters on site | SM6.4

Attenuation Tomography Analysis in the Val d’Agri Oilfield 

Martina Avella, Luca De Siena, Alexander Garcia, and Lucia Zaccarelli

The Val d’Agri basin in southern Italy is largest onshore hydrocarbon systems in Europe and, at the same time, one of the most seismically active sedimentary basins in the Apennines. This area appears as an ideal natural laboratory for investigating how fluids, rock damage and stress interact in the shallow crust thanks to the production and fluid injection that take place in this oilfield.
We analyze a dense local earthquake dataset recorded in the Val d’Agri area using seismic attenuation tomography. Attenuation is imaged with the MuRAT workflow, a Matlab algorithm that exploits multi-frequency measurements of direct and coda-wave amplitudes to recover three-dimensional distributions of scattering and absorption. These parameters are highly sensitive to fracture density, lithology, and fluid saturation, and therefore provide a physically meaningful view of the reservoir and fault system.
The resulting attenuation volumes allow us to identify zones of strong energy loss and high heterogeneity that may correspond to highly fractured, fluid-rich areas within the sedimentary cover and along major fault systems. Such features are particularly relevant in a georesource context, as they can act both as preferential fluid pathways and as mechanically weak volumes prone to seismic activation. Results of these analyses provide new light on the internal structure of the reservoir and its surrounding fault network, while also highlighting their interaction with industrial operations.
Overall, this work demonstrates how seismic energy attenuation tomography can provide a powerful framework for imaging fluid–fault interactions in active hydrocarbon systems. The results offer new insights into the processes controlling induced and triggered seismicity in the Val d’Agri basin and contribute to the development of geophysically informed strategies for sustainable resource exploitation and seismic risk management.

How to cite: Avella, M., De Siena, L., Garcia, A., and Zaccarelli, L.: Attenuation Tomography Analysis in the Val d’Agri Oilfield, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13919, https://doi.org/10.5194/egusphere-egu26-13919, 2026.

EGU26-14980 | ECS | Orals | SM6.4

Experimental characterization of urban-like scattering and attenuation from a dense nodal array: implications for seismic ground motion 

Malcon Humberto Celorio Murillo, Philippe Guéguen, Rita Touma, and Philippe Roux

Attenuation is a fundamental process of seismic wave propagation, yet its role in site–city
interaction remains poorly constrained and rarely quantified. In particular, un- derstanding
how buildings collectively dissipate seismic energy through scattering and absorption is essential
for assessing earthquake impact in urban areas. Numerical studies have recently introduced the
concepts of urban attenuation and urban mean free path to describe these processes. However,
observational evidence based on real data is still lack- ing, leaving open questions about how
such mechanisms manifest in practice.
In this study, we address this gap using the META-FORET experiment, in which a dense
pine forest is considered as a natural analogue of an urban environment. Trees act as distributed
reso- nant scatterers, allowing us to investigate urban-like scattering and attenuation processes
under well-characterized and repeatable conditions. We analyze both ambient noise and active
shot data to extract key ground motion parameters that are directly relevant to seismic hazard
assessment, including horizontal-to-vertical spectral ratios (H/V), spatial variability of ground
motion, wave attenuation and intensity indices. Passive data reveal frequency-dependent
scattering signatures around tree resonances (20 and 50 Hz), includ- ing perturbations of H/V
curves, reduced coherence and absorption.
Active shot analyses further show a systematic reduction of Arias intensity and a strong
increase in Trifunac duration within the forest compared to the open field, especially near
resonance frequencies. These observations indicate that resonant scatterers redistribute seismic
energy, reducing direct-wave amplitudes while enhancing coda wave durations.
This study provides the first experimental quantification of urban-like scattering and
attenuation from real seismic data. By bridging fundamental wave physics and ground motion
indicators, we propose a noise-based technique to characterize seismic wave atten- uation in
urban environments.

Keywords: urban-like scattering, wavefield coherence, absorption, seismic attenuation,
spectral ratios.

How to cite: Celorio Murillo, M. H., Guéguen, P., Touma, R., and Roux, P.: Experimental characterization of urban-like scattering and attenuation from a dense nodal array: implications for seismic ground motion, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14980, https://doi.org/10.5194/egusphere-egu26-14980, 2026.

EGU26-15304 | Posters on site | SM6.4

Attenuation Tomography of the Baihetan Reservoir: Separating Fluids from Fractures in Induced Seismicity 

Yansong Hu, Luca De Siena, Ruifeng Liu, Xinjuan He, and Lisheng Xu

Impoundment of the Baihetan Reservoir has triggered intense micro-seismicity, raising questions about the underlying hydro-mechanical drivers. While stress drop variations suggest fluid lubrication reduces effective normal stress, distinguishing fluid-saturated conduits from dry fracture networks remains challenging with traditional tomography. Standard attenuation imaging (Qt-1) inherently conflates scattering (structural heterogeneity) and intrinsic absorption (anelastic loss), obscuring the true physical state of the subsurface.

To resolve this, we apply Multi-Resolution Attenuation Tomography (MuRAT) to a dense local seismic array dataset. By utilizing Radiative Transfer Theory, we independently invert for scattering (Qsc) and absorption (Qi) attenuation coefficients. Our results reveal a distinct spatial decoupling of these mechanisms. Scattering anomalies (low-Qsc) correlate strongly with the surface traces of the Zemuhe and Xiaojiang fault zones, effectively imaging the pre-existing fracture network. In contrast, intrinsic absorption anomalies (low-Qi) are concentrated at depths of 5–10 km. These high-absorption features are spatially consistent with theoretical zones of fluid infiltration. By separating structural damage from fluid presence, we provide independent geophysical constraints that support fluid-diffusion hypotheses derived from source parameter analysis.

 

How to cite: Hu, Y., De Siena, L., Liu, R., He, X., and Xu, L.: Attenuation Tomography of the Baihetan Reservoir: Separating Fluids from Fractures in Induced Seismicity, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15304, https://doi.org/10.5194/egusphere-egu26-15304, 2026.

EGU26-17001 | Orals | SM6.4

Crustal Weakening by Mantle Upwelling in Southeastern Tibetan Plateau 

Haijiang Zhang, Jiachen Wang, Zengqian Hou, Bo Xu, Hao Guo, Clifford Thurber, and Robert van der Hilst

The conspicuous eastward expansion of the Tibetan Plateau is evident and uncontroversial from geological surface expressions and remote sensing, but the mechanisms that cause it have remained enigmatic. The extrusion has been attributed to ductile deformation of a weak crust. This is consistent with the discovery of mid-lower crustal low (seismic) velocity zones (LVZs), but the cause of crustal weakness and the origin and nature of the LVZs are debated, with competing hypotheses including channel flow from central Tibet, local fluid content, and mantle-derived processes. We present a high-resolution 3D seismic attenuation (Qp) model of the crust and uppermost mantle in southeastern Tibetan Plateau. Our results reveal high-attenuation anomalies in the middle-lower crust that overlap with previously imaged LVZs but extend across the Moho into the uppermost mantle. These anomalies correlate spatially with Cenozoic magmatism, mantle-derived helium isotope signatures, Zircon Hf-isotopes, and major strike-slip faults. This suggests that the crust in southeastern Tibetan plateau is weakened from below, possibly by upwelling induced by tearing of the subducted Indian slab.

How to cite: Zhang, H., Wang, J., Hou, Z., Xu, B., Guo, H., Thurber, C., and van der Hilst, R.: Crustal Weakening by Mantle Upwelling in Southeastern Tibetan Plateau, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17001, https://doi.org/10.5194/egusphere-egu26-17001, 2026.

EGU26-19330 | Posters on site | SM6.4

Magnitude and source spectra estimation using an elastic radiative transfer modelling of seismic wave-field attenuations: application to a French dataset.  

Grégoire Heller, Olivier Sèbe, Ludovic Margerin, Paola Traversa, Marie Calvet, and Jessie Mayor

Accurate magnitude estimates and reliable propagation models are essential for seismic hazard assessment. Unfortunately, the magnitudes of small earthquakes remain subject to significant uncertainties, primarily due to complex high-frequency propagation effects. Similarly, spatial variations in attenuation properties are crucial for refining ground motion models and reducing epistemic uncertainties in seismic hazard assessment. This study proposes (1) to map attenuation properties (scattering and absorption) in Metropolitan France using the radiative transfer theory of elastic waves, and (2) to simultaneously estimate source and site spectra through a generalized inversion. The recovered source spectra provide access to the moment magnitude Mw​, corner frequency fc​, and apparent stress σapp​.

We apply the entire inversion procedure to approximately 21,000 recordings from the EPOS-FR and CEA databases, including events with local magnitudes ML​ ranging from 2.0 to 5.9, and stations with hypocentral distances of less than 250 km. The estimated attenuation maps reveal strong spatial and frequency-dependent variations. Scattering dominates absorption at low frequencies (< 1 Hz), while absorption prevails at high frequencies. Strong scattering anomalies are concentrated in recent sedimentary basins at low frequencies and in deformed regions or deep sedimentary basins at medium and high frequencies. Conversely, Variscan units exhibit low scattering attenuation, especially at low frequencies. Absorption is highest in the French Alps and the western Pyrenees and lowest in the Armorican Massif. Concurrently, a catalog of 1,279 Mw​ magnitudes and 577 site terms is established for Metropolitan France. The obtained magnitudes are consistent with those in the unified Euro-Mediterranean catalog. Its comparison with the SI-Hex catalog highlights the importance for correcting the attenuation variations before extracting source parameters and especially the magnitude. The analysis of the apparent stress σapp​ reveals a moderate increase with the seismic moment M0​ (scaling exponent of 0.24±0.08), without any marked regional trend. Finally, we emphasize the importance of rigorously correcting for site effects, using reference stations on bedrock and of ensuring inter-event connectivity during the generalized inversion process through the existence of common stations across event records. The next step is to integrate this approach and related results in CEA seismic alert operational framework.

How to cite: Heller, G., Sèbe, O., Margerin, L., Traversa, P., Calvet, M., and Mayor, J.: Magnitude and source spectra estimation using an elastic radiative transfer modelling of seismic wave-field attenuations: application to a French dataset. , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19330, https://doi.org/10.5194/egusphere-egu26-19330, 2026.

EGU26-1143 | ECS | PICO | TS1.2

Strength Reversal in Recrystallisation: an EBSD-based Study in a Naturally Deformed Granitic Vein 

Anamitra Sikdar, David Wallis, and Santanu Misra

Strain partitioning in quartzo-feldspathic rock is closely related to the degree of phase mixing. Both quartz and feldspar tend to form the load-bearing framework (LBF) in naturally deformed rocks, provided there are softer phases such as mica, which behaves as the interconnected weak layer (IWL). In cases where mica is absent, the scenario becomes complicated. Quartz in augen gneisses often behaves as the IWL and feldspar takes the role of the LBF. However, the relative degree of weakening in deformed quartz and feldspar depends on their respective deformation mechanisms. As the mechanisms are different, there is a possibility of dissimilar weaking, followed by a strength reversal.

We have studied a deformed quartzo-feldspathic vein from the Bundelkhand Craton in central India. Despite being Archean, this craton experienced long hiatuses between deformation events, which makes the delineation between different events simpler. The sample we collected from this craton is the result of the latest stage of deformation. A high-temperature fluid entered through fractures and softened the granitic country rock. The fluid, being syn-tectonic, allowed the granitic vein to facilitate different deformation mechanisms in quartz and feldspars.

We investigated the crystal-plastic behaviour of quartz and two feldspars in the deformed vein via electron backscatter diffraction. The quartz crystallographic preferred orientation (CPO) and misorientation index (M) is strongest when quartz grains are adjacent to each other. There is no significant difference in CPO strength in feldspars when the proportion of similar neighbouring phases changes. Additionally, a monomineralic quartz layer exhibits a class 3 buckling fold, implying a higher competency than the adjacent matrix, which contains recrystallised feldspar grains. However, the microstructural evidence suggests that the parent feldspar porphyroclasts are stronger than the recrystallised monomineralic quartz bands. From the inverse pole figure of low-angle (2–10°) misorientation axes in quartz, prism <a> activity is observed which is dominant in the temperature range of 500–650°C. Hence, we infer a deformation temperature of at most 650°C, although it can be lower depending upon the water weakening as such weakening activates prism <a> at lower temperatures. Randomised CPO in feldspar suggests strain accommodation via diffusion creep, followed by grain boundary sliding mechanism might have operated in feldspars. These processes could result in greater softening than that in quartz, which deformed by dislocation creep. Isolated quartz grains existing in the triple junctions of feldspars are not part of such pure dislocation creep; rather, it is more likely that they are byproducts of albitic transformation reactions. Hence, higher strength in quartz is limited to the monomineralic bands, which are purely affected by dislocation creep in the deformed quartzo-feldspathic vein of the Bundelkhand Craton.

How to cite: Sikdar, A., Wallis, D., and Misra, S.: Strength Reversal in Recrystallisation: an EBSD-based Study in a Naturally Deformed Granitic Vein, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1143, https://doi.org/10.5194/egusphere-egu26-1143, 2026.

EGU26-4322 | ECS | PICO | TS1.2

Seismic twinning in monazite: Microstructural records of deep crustal earthquakes 

Renelle Dubosq, Alfredo Camacho, and Ben Britton

Earthquake records preserved in rocks provide key insights into the processes that govern crustal deformation and seismic energy dissipation. This manuscript presents new approaches for identifying mineralogical signatures of paleoearthquakes using advanced microstructural analyses, including electron backscatter diffraction (EBSD) and electron channeling contrast imaging (ECCI). These techniques enable observations from the millimetre to nanometre scale of features associated with plastic deformation, including crystal reorientation and deformation twinning. Here, we investigate deformation microstructures in monazite, a key geochronometer, with the aim of assessing the impact of deformation on geochronological interpretations, as deformation-induced crystallographic defects can act as high-diffusivity pathways leading to Pb loss. Understanding the deformational behaviour of monazite is therefore critical for interpreting geochronological data. We examine monazite from an eclogite facies mylonite in the Musgrave Province (central Australia) to elucidate mechanisms of seismic deformation under dry (<0.002 wt% H₂O), lower-crustal conditions. The studied monazite grain is directly cross-cut by a pseudotachylite vein, indicating that the observed microstructures formed during the associated seismic event. EBSD and ECCI analyses reveal crystal-plastic deformation in the form of twinning with three distinct orientations: 180° <100>, 180° <001>, and 95° <201>. The latter is associated with dynamic recrystallization via subgrain boundary rotation. ECCI further reveals nanometre-scale (<15 nm) porosity within both parent grains and twins. These microstructures are consistent with those reported in monazite deformed during impact events. Recent studies of shocked monazite have shown that deformation by twinning can liberate Pb during rupture of rare-earth-element–oxygen (REE–O) bonds, enabling rapid diffusion along crystallographic defects and complete expulsion from the crystal, effectively resetting the geochronometer. The new insight provided by these microstructural focussed observations likely accounts for the disparity of electron probe microanalysis (EPMA)-based geochronology on the same monazite grain, which yielded ages of 1309 to 691 Ma. Seismicity in the Musgrave Province is primarily associated with the Petermann Orogeny (~550 Ma), suggesting that the younger EPMA ages were partially reset as a result of the twinning. Our results demonstrate the potential for monazite to record and date seismicity, opening new avenues for reconstructing paleoearthquake histories from deep crustal rocks.

How to cite: Dubosq, R., Camacho, A., and Britton, B.: Seismic twinning in monazite: Microstructural records of deep crustal earthquakes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4322, https://doi.org/10.5194/egusphere-egu26-4322, 2026.

EGU26-4517 | ECS | PICO | TS1.2

The complex evolution of elasticity during metamorphic transformation 

Damien Freitas, James Gilgannon, Danielle Duggins, Ian Butler, Roberto Rizzo, Leonard Turpin, Bengang Chen, Christina Reinhard, and Neil Bourne

Prograde metamorphic reactions that reduce solid volume are common in subduction zones and orogenic settings [1]. These reductions are often linked to irreversible deformation such as viscous compaction and deep mantle earthquakes [2]. Viscous compaction involves permanent closure of reaction-generated porosity and fluid release, making porosity transient property of metamorphic reactions [3]. The pore closure observation is often linked to the intuitive loss of the elastic strength of the rock leading to permanent strains [4, 5], but these assumptions are very rarely demonstrated experimentally. In most cases, the nature of field relationships and the design of experiments do not allow for such an assessment to be made. Time-resolved in situ experiments enable the observation of a sample volume undergoing metamorphic transformation to check such assumptions at every stage of the reaction (loading, heating, cooling and unloading).

In this contribution, we provide preliminary visual and quantitative strain mapping during the metamorphic reaction cycle of a rock sample at various stress states and reaction extent.

Using Mjolnir, an X-ray transparent miniature triaxial deformation rig, we performed a series of gypsum (Ca2SO4·2H2O) dehydration experiments into bassanite (Ca2SO4·1/2H2O) at constant confining pressure of 20 MPa, pore fluid pressure (5 MPa) and subjected to similar temperature paths (up to 125ºC).  We used a series of differential stresses (radial, hydrostatic and axial principal stresses) to explore how the rock volume responds mechanically while also displaying different reaction fabrics (see [6]). This dehydration reaction produces a solid volume reduction of ~30% [4] enabling the investigation of the evolution of elasticity by unloading fully and partially transformed samples.

Using synchrotron microtomography at the I13-2 beamline of the Diamond Light Source (MG34156), we performed high resolution imaging (1.625 microns/ voxel edge) during gradual unloading to observe and quantify the elastic behaviour both using the mechanical data from the Mjolnir rig [7], sample dimensions (using stitched images; [8]) and digital volume correlation (DVC) techniques (Avizo). 

Our results show the complexity of strain distribution and partial preservation in metamorphic rocks with:

  • Significant elastic strain preservation during metamorphic reactions and its apparent minimisation during the ultimate stages of the reaction (textural “maturation” via pressure/solution).
  • Complex strain distribution influenced by bassanite anisotropy, sample fabric, geometry, and stress state.

These experiments enable to visualise in 4D the grain-scale development of a complex porous network during the reaction. It opens pathways to document the emergence of poro-elasticity (initial solid has very low porosity) and then the release of the elastic strains. This dataset further demonstrates the importance and the complexity of elasticity in metamorphic systems, with complex displacement vector fields under relatively simple boundary conditions.

References:

[1] Brown & Johnson (2019). https://doi.org/ https://doi.org/10.2138/am-2019-6956

[2] van Keken & Wilson (2023). https://doi.org/10.1186/s40645-023-00573-z

[3] Putnis (2015). https://doi.org/10.2138/rmg.2015.80.01

[4] Leclère et al. (2018). https://doi.org/10.1016/j.epsl.2018.05.005

[5] Llana-Fúnez et al. (2012). https://doi.org/10.1007/s00410-012-0726-8

[6] Gilgannon et al. (2024). https://doi.org/10.1130/G51612.1

[7] Butler et al. (2020). https://doi.org/ 10.1107/S160057752001173X

[8] Turpin et al. in prep

How to cite: Freitas, D., Gilgannon, J., Duggins, D., Butler, I., Rizzo, R., Turpin, L., Chen, B., Reinhard, C., and Bourne, N.: The complex evolution of elasticity during metamorphic transformation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4517, https://doi.org/10.5194/egusphere-egu26-4517, 2026.

EGU26-6735 | ECS | PICO | TS1.2

The material-independent effect of a differential stress on metamorphic kinetics 

James Gilgannon, Eilidh Vass Payne, Ian Butler, Damien Freitas, and Florian Fusseis

Deformation and metamorphism are fundamental processes that act synchronously throughout the Earth; however, their interaction remains unclear. Theoretical models predict that an applied tectonic stress has both a dramatic effect or no effect at all. While the small set of deformation experiments that document the interaction between reaction and deformation are either hard to compare or cannot provide the necessary time resolution to test the various theories. These disagreements of predictions and the gap in data invites new time-resolved experiments to be run that can probe details of model predictions and connect existing datasets from different materials deforming at a range of metamorphic conditions. To this end, we use state-of-the-art time-resolved synchrotron-based x-ray microtomography (4DSµCT) deformation experiments to map out the effect of a differential stress on the kinetics of the dehydration of polycrystalline gypsum samples. Our experiments are highly resolved in space (µm) and time (s), which allows us to track and contrast the emergence of the first small crystals (~100 µm3) and their growth through time in hydrostatic and differentially stressed conditions. We find that the kinetics of a metamorphic reaction are profoundly affected by the addition of deformational energy. Differentially stressed samples transform up to ~90% sooner than in the hydrostatic case, and reaction rates increase by a factor of ~5 with increasing differential stress. Importantly, our findings can be expanded to other published data for reactions occurring in the lower crust and the mantle to show that it is changes in the elastic strain energy that drive accelerated metamorphic kinetics. We find that, when we compare kinetic data from these different reactions and normalise the differential stress to each material’s yield strength, a trend emerges that shows stresses larger than the yield do not contribute to accelerating a reaction. Our results showcase the material-independent effect of a differential stress on metamorphic reactions and support theoretical models which place emphasis on the role of changes in stored energy. Current geodynamic models largely ignore the role of stored energy because it is assumed that it is not relevant at long time scales, our results show that its effect is important and should be accounted for when coupling deformation and metamorphism.

How to cite: Gilgannon, J., Vass Payne, E., Butler, I., Freitas, D., and Fusseis, F.: The material-independent effect of a differential stress on metamorphic kinetics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6735, https://doi.org/10.5194/egusphere-egu26-6735, 2026.

EGU26-7324 | PICO | TS1.2

Neutron and X-ray µ-tomography-based 3D imaging of alteration phases in faulted granodiorite at Nojima (Japan) 

Maxime Jamet, Fabien Baron, Daniel Beaufort, Baptiste Dazas, Patricia Patrier, Alessandro Tengattini, Romain Iaquinta, Mai-Linh Doan, Philippe Pezard, Benoît Gibert, and Linda Luquot

The study of the evolution of petrophysical properties and alteration of host rock in an active fault system is essential for understanding the mechanisms of deformation localization. The distribution of alterations is closely linked to fluid flow paths, while the formation of new deformation structures depends on the mechanical contrasts induced by these alterations. Our study focuses on granodiorite samples from a borehole drilled in 1996 at Hirabayashi by the Geological Survey of Japan, one year after the Nanbu-Kobe earthquake. Crossing the active Nojima fault, this borehole intersects the fault core at 625 m. The analyses include imaging of samples using neutron and X-ray microtomography (ILL – NeXT) and thin sections, as well as mineralogical quantification by X-ray diffraction (XRD). X-ray diffractograms on oriented slides and Rietveld analyses of XRD data acquired on disoriented powders reveal the presence of secondary mineral phases (e.g., montmorillonite, kaolinite, laumontite, siderite, ankerite), representative of different fluid-rock interaction conditions during the exhumation of the massif. Their proportions, which increase as they approach the fault, reach more than 30% of the volume of a sample at 625 m. Whereas X-ray µ-tomography imaging allows us to observe density contrasts within the samples (e.g., mineral phases and fracture network). On the other hand, neutron imaging allows us to observe the distribution of hydrated mineral phases due to the high neutron absorption coefficient of hydrogen (e.g. for 25 meV neutrons, hydrogen attenuation is 3.44 vs 0.17 and 0.11 for oxygen and silicon, respectively). Neutron and X-ray image registration in the same reference frame allows us to perform joint image segmentation, using gaussian-mixture-model to quantify uncertainties, based on the neutron and X-ray coefficients of absorption of the pre-identified mineral phases. The volumes segmented in this way enable us to (i) quantify in a non-destructive way the volume of secondary mineral phases present in the samples along the fault damage profile and (ii) obtain their spatial distribution and assess the anisotropies of distribution in relation to the deformation structures. This work will subsequently enable us to understand the impact of both the distribution of secondary mineral phases and the network of microfractures on the evolution of the petrophysical and mechanical properties of a seismogenic fault.

How to cite: Jamet, M., Baron, F., Beaufort, D., Dazas, B., Patrier, P., Tengattini, A., Iaquinta, R., Doan, M.-L., Pezard, P., Gibert, B., and Luquot, L.: Neutron and X-ray µ-tomography-based 3D imaging of alteration phases in faulted granodiorite at Nojima (Japan), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7324, https://doi.org/10.5194/egusphere-egu26-7324, 2026.

EGU26-7733 | PICO | TS1.2

A new concept of Messinian Salinity Crisis based on physical properties from the IODP Exp.402 in the Tyrrhenian Sea 

Maria Filomena Loreto, Marco Ligi, Irina Y. Filina, Noriaki Abe, Brandon D. Shuck, Philippe A. Pezard, Emily R. Estes, Alberto Malinverno, Cesar R. Ranero, Lining Yang, and Nevio Zitellini

During the International Ocean Discovery Program (IODP) Expedition 402 in the Tyrrhenian Sea, two of the six drilled sites, the U1613 and U1617, were located on the thinned continental crust of the Cornaglia and Campania terraces, where the deposition of evaporites during the Messinian Salinity Crisis (MSC) had been imaged with seismic data. Expedition 402 recovered Messinian evaporites beneath a relatively thin sedimentary cover at both drill sites. At Site U1613, the Messinian section is extremely thin (a few meters only). In contrast, at Site U1617, a complete 102 m-thick evaporitic sequence ranging from gypsum-enriched terrigenous sediments through anhydrite to halite layers was sampled. This scientific drilling site is the only one in the Mediterranean that penetrated the complete Messinian evaporitic sequence, providing a unique opportunity to study the properties of the so-called Upper, Mobile and Lower units. A series of physical property measurements was performed on these cores on board of the JOIDES Resolution drillship, including P-wave velocity, density, magnetic susceptibility, natural gamma ray and thermal conductivity. In addition, we collected representative discrete samples to measure P-wave velocity (Vp), bulk density, grain density and porosity. These data allowed us to analyze the sealing properties of the halite unit and its interaction with salt-induced tectonics. Furthermore, from Vp and density used as input to calculate reflection coefficients, we generated a 1D synthetic seismogram at Site U1617. We compared this synthetic seismogram with the multi-channel seismic data acquired across the drill site, namely the Medoc 6 line. These new data allowed us to compare the Messinian units recovered in situ with multichannel seismic data and thereby revise seismic interpretation of these units. Thanks to the unique opportunity offered by the IODP Expedition 402, we now have reliable data on the physical properties of Messinian evaporites and we are able to provide new constraints on the interpretation of Messinian facies.

How to cite: Loreto, M. F., Ligi, M., Filina, I. Y., Abe, N., Shuck, B. D., Pezard, P. A., Estes, E. R., Malinverno, A., Ranero, C. R., Yang, L., and Zitellini, N.: A new concept of Messinian Salinity Crisis based on physical properties from the IODP Exp.402 in the Tyrrhenian Sea, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7733, https://doi.org/10.5194/egusphere-egu26-7733, 2026.

EGU26-7751 | PICO | TS1.2

In situ observation of faulting in olivine at high pressures and high temperatures using high-flux synchrotron X-rays 

Tomohiro Ohuchi, Yuji Higo, Noriyoshi Tsujino, Sho Kakizawa, Hiroyuki Ohsumi, and Makina Yabashi

The mechanisms of intraslab earthquakes at depths of > 40 km are fundamentally different from those of shallow earthquakes because the frictional strength of silicate rocks is proportional to the confining pressure. To understand the process triggering intraslab earthquakes, many experimental studies on faulting of slab-forming rocks have been conducted at upper mantle pressures. Previous studies have revealed that shear localization induced by dehydration of hydrous minerals (e.g., Okazaki & Hirth, 2016) or adiabatic shear heating (e.g., Kelemen & Hirth, 2007) is essential for the occurrence of faulting at high pressures. Although acoustic emission (AE) monitoring technique for D-DIA apparatuses enabled us to discuss the process of microcracking at high pressures, mechanical behavior at the onset of faulting is still unclear due to low time-resolution stress/strain measurements using synchrotron X-rays. The cause of bottleneck in stress/strain measurements is a long exposure time required for the acquisition of a two-dimensional X-ray diffraction pattern of minerals. Considering that the timescale of stress drop associating faulting is on the order of 0.01 sec (e.g., Okazaki & Katayama, 2015), a significant improvement for time resolution of stress/strain measurements is required. To improve the time resolution of stress/strain measurements, we installed a series of new devices at BL15XU, SPring-8.

We conducted in situ triaxial deformation experiments on olivine aggregates at pressures of 1-3 GPa and temperatures of 700-1250 K under nominally dry conditions using a D-DIA apparatus, installed at BL15XU, SPring-8. Two-dimensional radial X-ray diffraction patterns and radiographic images were alternately acquired by adjusting sizes of the incident slit and operating a flatpanel detector and a CCD camera using a high-flux pink beam (energy 100 keV) from an undulator source (0.2 s of exposure time for both ones). Pressure and differential stress were determined from the d-spacing of olivine. Strains of deforming samples were evaluated from the distance between platinum strain markers. AEs were recorded continuously on six sensors glued on the rear side of the 2nd-stage anvils, and three-dimensional AE source location were determined.

Stress increased with strain at the beginning of sample deformation, and it reached the yielding point at strains of ~0.1 or less. AEs from the deforming sample were detected when stress exceeded ~1 GPa and the amplitude of AE is positively correlated with the magnitude of stress. At strains higher than 0.1 (i.e., beyond the yielding point), both softening (i.e., decrease in stress and/or increase in strain rate) and a decrease in AE rate were observed prior to the occurrence of faulting. Faulting was observed at 880-1150 K. Most of unstable slips proceeded within 1 s and associated a sudden stress drop (~0.5 GPa) and temporal radiation of large AEs. In contrast, neither stress drops nor AEs were associated with a few “aseismic” unstable slips. Differential stress continuously increased when stable slip proceeded and the stable slip was terminated by the occurrence of another unstable slip. Our observations suggest that unstable slips can be divided into two types (i.e., seismic and aseismic ones) under the P-T conditions of shallow subducting slabs.

How to cite: Ohuchi, T., Higo, Y., Tsujino, N., Kakizawa, S., Ohsumi, H., and Yabashi, M.: In situ observation of faulting in olivine at high pressures and high temperatures using high-flux synchrotron X-rays, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7751, https://doi.org/10.5194/egusphere-egu26-7751, 2026.

EGU26-7796 | PICO | TS1.2

Abnormal grain growth in carbonate samples from the North Anatolian Fault: Microstructural evidence of the seismic cycle 

Yuval Boneh, Tsafrir Levi, Perah Nuriel, and Ram weinberger

Evidence for the nature of fault slip across the seismic cycle is hard to decipher. Fault-related deformation near the fault surface develops over the seismic cycle, characterized by rapid coseismic slip and intense deformation, followed by slower interseismic slip and stress accumulation. While considerable focus has been placed on characterizing deformation through fracturing and mesoscale structures, the analysis of grain-scale plastic processes has been largely neglected. However, transient temperature increases due to frictional heating, combined with the ability of calcite-bearing rocks to deform plastically at relatively low temperatures, suggest that microstructural damage and subsequent recovery processes could leave diagnostic evidence in carbonate fault rocks. Indeed, Pozzi et al. (2019) demonstrated that shearing gouge at seismic rates (~1 m/s) develops a crystallographic preferred orientation (CPO), accompanied by grain growth and sintering. These observations, however, were confined to nanometer-scale grains, localized at the fault surface.

Here, we present a detailed microstructural analysis of carbonate samples from the North Anatolian Fault Zone. We used Electron Backscatter Diffraction to map the calcite grains' orientations and characterize intragrain deformation and grain-boundary morphologies. We identify three distinct layers extending from the fault surface to a distance of ~4 mm. Layer I, with a thickness of tens of µm to 0.5 mm, exhibits predominantly angular grains with grain sizes ranging from unresolved (<1 µm) to tens of µm. Layer II, with a thickness of 0-200 µm, is comprised of small equant grains (1-5 µm) and some larger grains (10-30 µm), characterized by wavy grain boundaries, suggesting active grain boundary migration. No CPO was observed in layers I and II. Layer III, with a thickness of ~2-3 mm, contains large grains (hundreds of µm) that can be divided into two populations of grains. Rounded grains with wavy grain boundaries indicate the progressive consumption of smaller grains. At the core of the layer, grains contain faceted boundaries and are elongated parallel to the fault surface. This layer is the only one to exhibit a distinct CPO with the c-axis oriented normal to oblique to the slip surface. Importantly, the large grains in layer III also comprise small, isolated ‘islands’ of finer grains.

We infer that deformation mechanisms vary systematically with distance from the fault surface. Layer I records cataclastic flow at the fault surface, whereas layer II, characterized by very small grain sizes, exhibits shearing by grain boundary sliding that resulted in grains with low intragrain misorientation and the absence of CPO. The most striking microstructural record is preserved in layer III, which initially shows strong evidence for recovery processes by abnormal grain growth. We propose that this latter process occurred during or immediately after coseismic frictional heating, resulting in the consumption of previously deformed grains, which maintains the CPO record of deformation and provides a microstructural record of the seismic cycle at millimeter-scale distances from the fault surface.

Pozzi, et al., 2019. Coseismic ultramylonites: An investigation of nanoscale viscous flow and fault weakening during seismic slip. Earth and Planetary Science Letters.

How to cite: Boneh, Y., Levi, T., Nuriel, P., and weinberger, R.: Abnormal grain growth in carbonate samples from the North Anatolian Fault: Microstructural evidence of the seismic cycle, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7796, https://doi.org/10.5194/egusphere-egu26-7796, 2026.

EGU26-8362 | PICO | TS1.2

Nano- and micro-scale imaging of rocks with X-ray ptychography 

Christoph E. Schrank, Michael W. M. Jones, Cameron M. Kewish, Grant A. van Riessen, Gerard Hinsley, Alfons Berger, Marco Herwegh, Berit Schwichtenberg, Nicole D. Bishop, Daryl Howard, Andrew D. Langendam, and David J. Paterson

X-ray ptychography is a lensless, coherent-diffraction imaging technique developed over the last 20 years that affords 10-nm resolution for optically thick specimens1. It reconstructs the optical transmission function (OTF) of a sample from raster-scanned overlapping 2D transmission diffraction patterns through iterative phase retrieval algorithms1,2. The OTF projects the refractive index of the sample along the incident beam and thus quantifies the phase shift and amplitude attenuation of the transmitted beam2, which in turn relate to the projected electron density of the specimen. X-ray ptychography is therefore an ultramicroscopy technique that is very well suited to mapping nano- and micron-sized objects with significant density differences relative to the bulk such as pores and dense accessory minerals.   

In this contribution, we present a primer for the application of X-ray ptychography to nano- and micro-scale studies of rocks. First, we illustrate the underlying physical principles that guide the data processing and interpretation of ptychographs. Then, we show exemplary applications to a wide range of rock samples (e.g., seismogenic brittle fault rocks, mylonites, veins, shale, and micrite) imaged at the XFM beamline of the Australian Synchrotron3 over the last 5 years4,5. Application examples include the measurement of sample surface roughness, imaging of cracks and pores, 3D porosity measurements, and the detection of buried accessory phases.

References

1          Pfeiffer, F. X-ray ptychography. Nature Photonics 12, 9-17, doi:10.1038/s41566-017-0072-5 (2018).

2          Wittwer, F., Hagemann, J., Brückner, D., Flenner, S. & Schroer, C. G. Phase retrieval framework for direct reconstruction of the projected refractive index applied to ptychography and holography. Optica 9, 295-302, doi:10.1364/OPTICA.447021 (2022).

3          Howard, D. L. et al. The XFM beamline at the Australian Synchrotron. Journal of Synchrotron Radiation 27, 1447-1458, doi:doi:10.1107/S1600577520010152 (2020).

4          Jones, M. W. M. et al. High-speed free-run ptychography at the Australian Synchrotron. Journal of Synchrotron Radiation 29, 480-487, doi:https://doi.org/10.1107/S1600577521012856 (2022).

5          Schrank, C. E. et al. Micro-scale dissolution seams mobilise carbon in deep-sea limestones. Communications Earth & Environment 2, 174, doi:10.1038/s43247-021-00257-w (2021).

How to cite: Schrank, C. E., Jones, M. W. M., Kewish, C. M., van Riessen, G. A., Hinsley, G., Berger, A., Herwegh, M., Schwichtenberg, B., Bishop, N. D., Howard, D., Langendam, A. D., and Paterson, D. J.: Nano- and micro-scale imaging of rocks with X-ray ptychography, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8362, https://doi.org/10.5194/egusphere-egu26-8362, 2026.

EGU26-9434 | ECS | PICO | TS1.2

Localized dehydration of antigorite during experimental deformation at subduction zone conditions 

Danielle Silva Souza, Marcel Thielmann, Florian Heidelbach, and Daniel Frost

Dehydration embrittlement is the dominant mechanism proposed to explain deep-focus earthquakes between 100–350 km in depth. Antigorite dehydration was extensively investigated in previous experimental studies, which demonstrated contrasting results regarding the seismic potential of antigorite dehydration. Additionally, microstructural aspects of antigorite dehydration and their implications for deep seismicity are scarce. Localized dehydration, on the other hand, might generate strain weakening, potentially leading to failure at depths relevant to deep earthquakes. Localized antigorite dehydration is demonstrated to occur in nature and the laboratory; however, it is not clear if this is a passive or dynamic process.

To better understand the micro-mechanisms of localized antigorite dehydration, we conducted high-pressure, high-temperature experiments under isostatic and non-isostatic conditions. Experiments were run at 3 GPa and temperatures within and above the antigorite stability field (530 °C–800 °C). Antigorite cores with 2 mm diameter were mounted in cubic assemblies and deformed in a 6-ram multi-anvil press at the Bayerisches Geoinstitute. Pure shear deformation was applied by inserting one pair of anvils while simultaneously removing the remaining two pairs orthogonal to it.

Results show that isostatic dehydration of antigorite at 3 GPa starts at ~530 °C and completes at ~800 °C. Localized dehydration occurs in isostatic and non-isostatic conditions within the antigorite stability field. It is enhanced during deformation experiments, resulting in the formation of nanocrystalline veins and networks containing olivine and pyroxene. These results demonstrate that localized dehydration might occur through passive and dynamic processes with the development of different microstructures.

How to cite: Silva Souza, D., Thielmann, M., Heidelbach, F., and Frost, D.: Localized dehydration of antigorite during experimental deformation at subduction zone conditions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9434, https://doi.org/10.5194/egusphere-egu26-9434, 2026.

EGU26-9614 | ECS | PICO | TS1.2

Trace element mapping in vein calcite with synchrotron XFM: implications for U-Pb geochronology 

Ismay Vénice Akker, Christoph E. Schrank, Michael W. M. Jones, Daryl Howard, Lorenzo Tavazzani, and Luiz Morales

U-Pb geochronology via Laser Ablation-Inductively Coupled Plasma-Mass Spectrometry (LA-ICP-MS) is a fast and reliable method for in-situ dating of calcite that is used across disciplines in earth science. However, the heterogeneous distribution of U (and Pb) in individual calcite crystals represents a yet unmitigated challenge and identifying zones of sufficiently high U concentrations that can provide precise constraints on timing of calcite precipitation is an inefficient “hit or miss” process. Moreover, it is challenging to confirm that targeted domains of a calcite crystal retain their pristine geochemical signature, given the range of post-crystallization dissolution-reprecipitation and solid diffusion processes that can affect this mineral. There is thus an urgent need to understand the spatial and temporal mechanisms of U incorporation and mobilization in calcite to ultimately improve this key geochronological tool. To determine where specific trace elements are located within calcite crystals, investigate how they are incorporated during crystal growth and how they are affected by post-crystallization fluid-assisted deformation processes, we applied Synchrotron X-Ray Fluorescence Microscopy (XFM) with emphasis on U mapping, Electron Backscatter Diffraction (EBSD), and LA-ICP-MS to a set of calcite veins. Samples were collected from drillcores through the Middle and Upper Jurassic carbonates and marls (max. 85°C) in the Neogene Molasse Basin in central northern Switzerland. By combining high-resolution trace element maps with information on the crystal lattice structure of calcite we show two main textural types of trace element distributions within syntaxial calcite veins: 1) oscillatory crystal growth zonations that reflect preferential incorporation of trace elements into structurally different growth steps and faces of growing calcite crystals during growth and, 2) complete overprint of the initial growth zonation upon potential secondary fluid infiltration and trace element replacement. The anti-correlation between Fe, Mn and Sr, U demonstrates the role of kinetic factors during trace element partitioning between fluid and calcite, pointing to the inhibition of Fe incorporation at higher growth rates. Where the Sr uptake during calcite growth is generally enhanced with growth rate. The results of this project give valuable insights in the complexity of fluid overprint during multi-staged deformation cycles in the modification of trace elements in calcite, with clear implications for the applicability and reliability of U-Pb geochronometer in calcite.

How to cite: Akker, I. V., Schrank, C. E., Jones, M. W. M., Howard, D., Tavazzani, L., and Morales, L.: Trace element mapping in vein calcite with synchrotron XFM: implications for U-Pb geochronology, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9614, https://doi.org/10.5194/egusphere-egu26-9614, 2026.

EGU26-9678 | ECS | PICO | TS1.2

An experimental investigation of dynamic recrystallisation processes and their influence on the mechanical properties of natural rock salt samples 

Evangelos Dialeismas, Hans de Bresser, Suzanne Hangx, and Jan ter Heege

Salt caverns are formed in the subsurface during solution mining of salt. After the end of salt production, caverns need to be safely abandoned or may be repurposed for storage of energy carriers such as hydrogen. Salt caverns locally disturb subsurface stresses, leading to creep of the surrounding rock salt. Creep can cause cavern convergence at depth and may result in surface subsidence, with consequences for infrastructure and public safety. Accurate forecasting of cavern stability during abandonment or assessment of suitability for storage requires a deep understanding of the grain scale deformation mechanisms and processes controlling rock salt strength and creep rate. For rock salt, important deformation mechanisms are dislocation creep and pressure solution creep. Laboratory experiments have shown that dynamic recrystallization (DRX) associated with dislocation creep can be activated and contribute to mechanical weakening. However, the weakening effect of DRX is not included in engineering constitutive laws used in salt cavern numerical models. These laws are commonly based on low-strain laboratory experiments, where the influence of DRX is limited, and microstructural data are relatively rarely reported. The aim of this study is to experimentally investigate the dominant DRX process in deforming natural rock salt and its effect on the mechanical behaviour.

Lab experiments have been carried out on natural wet salt samples from the Zechstein formation. We conducted constant strain rate experiments using a triaxial compression apparatus. Experiments were performed at a confining pressure of 20 MPa and a temperature of 125 °C, using constant displacement rates corresponding to strain rates of approximately 5 × 10⁻⁵ s⁻¹ and 5 × 10⁻⁷ s⁻¹, up to 30–40% axial strain. After the experiment, all samples were studied using optical microscopy. Electron backscatter diffraction (EBSD) analysis was performed on the starting material and on two deformed samples, one from each strain-rate condition.

For all samples, we observed an initial transient creep stage followed by a quasi-steady state stage. The transition to quasi-steady occurred at a strain of about 10% for samples deformed at a strain rate of ~5 × 10-7 s-1. For samples deformed at the faster strain rate of ~5 × 10-5 s-1, continuous hardening occurred up to axial strains of 30%, with a gradually decreasing hardening rate approaching steady state. Light optical and EBSD microstructural analysis revealed grains with a dense substructure including subgrain walls, euhedral shape grains with low to no substructure, and grains with irregular shaped grain boundaries including bulges. We infer that the dominant deformation mechanism in the tested natural samples was dislocation creep, providing sufficient local differences in dislocation density to activate DRX dominated by grain boundary migration processes. DRX led to rheological weakening and quasi-steady deformation. We are working on robust understanding of the parameters controlling DRX as this is essential to evaluate the zones prone to weakening by DRX around salt caverns.

How to cite: Dialeismas, E., de Bresser, H., Hangx, S., and ter Heege, J.: An experimental investigation of dynamic recrystallisation processes and their influence on the mechanical properties of natural rock salt samples, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9678, https://doi.org/10.5194/egusphere-egu26-9678, 2026.

EGU26-11242 | ECS | PICO | TS1.2

High-resolution microstructural study of calcite crystals precipitated through bio-cementation under different conditions 

Marilyn Sarkis, Carsten Detlefs, Michela La Bella, Antoine Naillon, Christian Geindreau, Fabrice Emeriault, Yves Watier, James A. D. Ball, and Can Yildirim

Bio-cementation is a new, environmentally-friendly soil-reinforcement process. It is used for civil engineering purposes, such as the fabrication of construction materials, as well as the preservation of monuments. This process uses bacterial activity, mainly that of Sporosarcina Pasteurii, that is capable of  hydrolysing the urea present in the medium, leading to the precipitation of CaCO3 (calcite) crystals between sand grains, therefore binding them together, and reinforcing the soil. The macro and micro (contact scale) mechanical properties of bio-cememted sand have been extensively studied. However, the microstructure of the precipitated calcite crystals remains undiscovered, which induces mechanical differences under different conditions of cementation. The goal of this study is to investigate the microstructure of biogenic calcite, issued from bio-cementation of sand, and how it varies under different cementation conditions. For this, high resolution synchrotron diffraction imaging at the ESRF was performed, utilizing scanning 3DXRD (s-3DXRD) on ID11 and Dark-Field X-ray Microscopy (DFXM) on ID03. For this, the main experiment was performed on three samples that consist of 3D printed resin cells in which cementation was performed under different conditions, by varying the substrate on which the calcite was grown (between sand grains and glass beads), as well as varying the salinity of the medium. After each cementation cycle, and for each sample, layer measurements were acquired using s-3DXRD. A significant difference was observed between the sand and glass bead cases: the precipitated crystals on the glass beads were much smaller than those precipitated on the sand grains. DFXM measurements showed defects that are only present in the case of high concentration of NaCl in the medium, which could potentially alter the mechanical properties of the material. These two complementary techniques allowed for an in-depth study of the microstructure of the precipitated calcite crystals.

How to cite: Sarkis, M., Detlefs, C., La Bella, M., Naillon, A., Geindreau, C., Emeriault, F., Watier, Y., Ball, J. A. D., and Yildirim, C.: High-resolution microstructural study of calcite crystals precipitated through bio-cementation under different conditions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11242, https://doi.org/10.5194/egusphere-egu26-11242, 2026.

EGU26-11671 | PICO | TS1.2

Olivine Deformation: to B Slip or not to B Slip, that is the Question 

John Wheeler, Simon Hunt, Alexander Eggeman, Jack Donoghue, Ali Gholinia, Yizhe Li, Evan Tillotson, and Sarah Haigh

When deformed by dislocation creep the dominant slip (Burgers) vectors of olivine dislocations are parallel to [100] or [001]. Dislocations with an [010] Burgers vector component (b dislocations) have been recorded rarely. Here we show an experimentally deformed olivine sample has a substantial population (17%) of b dislocations. Electron Backscatter Diffraction maps of crystal orientations provided information on dislocations from the orientation gradients. Maps show the b dislocations form subgrain walls like those formed by other dislocation types and are interpreted to form similarly by glide and climb, so b dislocations are mobile. To confirm our approach, we used EBSD maps to select an area for Transmission Electron Microscopy imaging, down to an atomic scale image of a b dislocation. Our sample was deformed within range of subduction zone conditions; our approach can be used to investigate the scale and conditions of b slip in the mantle more widely.

How to cite: Wheeler, J., Hunt, S., Eggeman, A., Donoghue, J., Gholinia, A., Li, Y., Tillotson, E., and Haigh, S.: Olivine Deformation: to B Slip or not to B Slip, that is the Question, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11671, https://doi.org/10.5194/egusphere-egu26-11671, 2026.

EGU26-11961 | PICO | TS1.2

Combining X-ray absorption and Induced Polarization Spectroscopies for in situ monitoring of Cation Exchange in clay materials 

Alexandra Courtin, Damien Jougnot, Erwan Paineau, Damien Roy, Delphine Vantelon, Augustin Dallaporta, and Emmanuel Léger

The Cation Exchange Capacity (CEC) of clay minerals has been extensively studied in wide applications / purposes, using various imaging techniques to highlight changes of the clay sheet chargeability. Among the clay minerals, swelling clays such as smectite or vermiculite are particularly interesting regarding their adsorption-desorption properties strongly related to their high CEC (80-150 to 100-150 meq/100g respectively). To better monitor and predict cation exchange processes, the CEC has been investigated by different methodological approaches, including X-ray absorption spectroscopy (XAS) and geoelectrical methods. The Spectral Induced Polarization (SIP) is particularly well designed to quantify CEC because its complex conductivity measurements (in phase and quadrature) characterizes the electrical conduction of charge carriers (liquid) and the polarization phenomenon resulting from the local accumulation of electrical charge carriers in the porous medium (mineral interface).

The aim of this work is to investigate in situ how K cations are incorporated within the interlayer of a Ca-montmorillonite by coupling XAS and SIP experimental methods. This novel approach brings multi-scale information at the atomic and clay-sheet levels, providing new insights on enhancing the understanding of CEC mechanisms in terms of time and space and our ability to monitor it with SIP. The experiment was carried out on LUCIA (Soleil synchrotron), at the low energy of potassium K-edge with a microbeam size (2.5 x 2.5 µm²).

We used a 1.7 mm3 cell filled with 0.1 g of Ca-Montmorillonite isolated in a 0.8 µm sieve to avoid flushing of the clay sample during the experiment. The cell was subjected to a solution flux of a few cc per minute with 4 different KCl salinities (0.01, 0.05, 0.1, 1 M of KCl).  In situ SIP spectra are compared with XAS to conjointly monitor the CEC exchange at different scales. Preliminary results are shown to test-proof the methods as a new in situ / in operando cross-scale methods for CEC spatio-temporal characterization. Overall,this work is the first step of a technological development project, merging the approaches of geophysicists, mineralogists and physicists to monitor in real time the cation exchange processes of a Ca-montmorillonite by K in swelling clay minerals. 

How to cite: Courtin, A., Jougnot, D., Paineau, E., Roy, D., Vantelon, D., Dallaporta, A., and Léger, E.: Combining X-ray absorption and Induced Polarization Spectroscopies for in situ monitoring of Cation Exchange in clay materials, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11961, https://doi.org/10.5194/egusphere-egu26-11961, 2026.

The evolution of orogens is steered by complex deformation processes that act at several crustal levels, evolving over time from syn- to post-orogenic. Investigating how strain and deformation localize in the ductile domains of the deep crust and brittle domains of the shallow crust can improve our understanding of the processes ultimately controlling the exhumation of deeply seated rocks. Within this framework, the Sestri-Voltaggio Zone (SVZ) of the Italian Ligurian Alps provides a record of rocks and structures attesting to the complete subduction-exhumation cycle during the Europe-Adria convergence. The SVZ is a mature fault zone characterized by a polyphase tectonic evolution and a high lithological variability, which tectonically juxtaposes high-pressure (HP) metamorphic units to non-metamorphic rocks. It also represents an abrupt structural-metamorphic boundary between the Voltri Massif (an eclogitic domain defining a southern culmination of the Western Alps) to west, and the Northern Apennines units (anchi-metamorphic or non-metamorphic) to east. The exhumation processes that led to the current outcropping units of the SVZ occurred following a multi-stage progression from early ductile to later brittle conditions. However, open questions remain reflecting the generalized lack of systematic descriptions of structural fabrics formed during the exhumation-related events of the SVZ units. In this recently launched study we further explore the exhumation mechanisms of the SVZ by investigating how the pre-existing metamorphic fabrics helped localize the brittle deformation that occurred at later stages at shallow crustal levels. Preliminary field observations and structural analyses document N-S to NNE-SSW-striking brittle faults separating lenses of HP-mafic (metagabbros and metabasalts) and carbonate lithotypes from the enveloping phylladic schists and serpentinites. The enclosed lenses exhibit a pervasive internal schistosity that strikes either parallel or at high angle to the orientation of the main SVZ boundaries. By mapping the orientation of the rock fabric as a function of distance, perpendicular to the main tectonic boundaries, it is possible to identify systematic geometric trends between the metamorphic foliations and the bounding brittle faults. Within the matrix, the metamorphic schistosity wraps around the lenses, varying both in strike and dip. Brittle faults, with dominant oblique kinematics, are characterized by a double behavior: they truncate the metamorphic schistosity when approaching massive lenses; but they tend to rework the schistosity within the phylladic matrix. The overall structural record of the investigated units highlights the distribution of strain localization within the deeply exhumed units, suggesting a distinction between episodic vs. progressive transition from ductile to brittle during exhumation. In this sense, the SVG can be considered a useful example of the deformation history of the Western Alps-Northern Apennines tectonic junction, with noteworthy implications on the first-order mechanisms leading to the exhumation of deeply seated rocks.

How to cite: Generi, A., Viola, G., and Vignaroli, G.: Characterizing ductile-to-brittle exhumation of polymetamorphic units along the Sestri-Voltaggio Zone (Ligurian Alps, Italy)., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13049, https://doi.org/10.5194/egusphere-egu26-13049, 2026.

Microstructural investigations of halite are essential for understanding deformation mechanisms relevant to salt tectonics and underground storage applications, including radioactive waste disposal and salt caverns. However, the identification of subgrain boundaries, dislocation structures, acting creep mechanisms and fluid-related features remains challenging due to the optical transparency and inherently low defect contrast of halite. Gamma decoration provides a powerful solution by inducing radiation-related colour centers that selectively highlight lattice defects and deformation structures.

At the Forschungs-Neutronenquelle Heinz Maier-Leibnitz (FRM II, TUM), gamma decoration has been implemented since over a decade, recently we re-established and systematically optimized it using older spent fuel elements characterized by comparatively low dose rates. This contribution focuses on methodological developments and parametric studies that enable reliable gamma decoration under these conditions, extending the applicability of the technique beyond high-dose irradiation facilities.

We present results from controlled irradiation experiments on halite thin sections covering a wide range of total doses, irradiation times, and temperatures, combined with post-irradiation optical microscopy, spectroscopy, and digital colorimetry to quantify and optimize suitable optical contrast. Our experimental results from long-term irradiations are compared with theoretical models describing dose-rate-dependent radiation effects on defect formation in natural rock salt. This parametric approach allows identification of threshold conditions required for effective defect visualization, as well as optimization strategies to compensate for reduced dose rates, including extended irradiation times and temperature control.

These results establish gamma decoration at FRM II as a robust and versatile experimental method for salt-rock research, providing a valuable link between laboratory testing, microstructural analysis, and mechanical modelling, and ensuring continued applicability of this technique with ageing irradiation infrastructure.

How to cite: Hutanu, V., Li, X., and Schmatz, J.: Gamma decoration at FRM II: recent optimisations and parametric studies for microstructural investigations of halite, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13462, https://doi.org/10.5194/egusphere-egu26-13462, 2026.

EGU26-13669 | PICO | TS1.2

Spatial phase distribution and deformation processes 

Rüdiger Kilian

Spatial phase distributions can be grouped into random, clustered or anticorrelated/distributed based on the probability to encounter a given nearest neighbour. This property can also be probed with respect to intervals of directions, frequently revealing an anisotropy in the spatial phase distribution. In this study, several high temperature ultramylonites with variable composition from felsic to ultramafic as well as coarse grained deformed rocks (e.g. eclogite from Münchberg, Germany) were investigated. Measurements of phase distribution anisotropy frequently manifest in a pronounced direction of phase clustering and one direction of anticorrelation. Especially in the investigated ultramylonites but also in deformed eclogites and amphibolites, those two directions are found not to be orthogonal and not to coincide with finite strain axes (as far as manifested by foliation and stretching lineation). Clustering phases (e.g. qtz, plg or grt, depending on the rock type) form stacks antithetically tilted against the sense of shear. These stacks are separated by phases such as kfs, bt or cpx. Below a certain volume threshold of the stack-forming phase, stacking is not observed.

In addition to the phase distribution, truncated chemical zonations and/or indications of directed growth are frequently observed. On the other hand, there is a lack of microstructures which can reasonabley be associated with steady state dislocation creep.

It is suggested that the observed microstructures in combination indicate deformation by a mechanism best described by dissolution-precipitation accommodated granular flow (or "diffusion creep" in the broadest sense). Stack-forming phases undergo mostly rigid-body rotation and translation temporarily forming transient force chains before being disintegrated again. Since these stacks can be observed in the rock record, the residence time in the force chain position must be greater than in a randomly distributed position, compatible with jamming of particles during granular flow.

The presence of this particular type of anisotropic spatial phase distribution may not only serve as a shear sense indicator but could in general be useful for the identification of deformation mechanisms.

How to cite: Kilian, R.: Spatial phase distribution and deformation processes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13669, https://doi.org/10.5194/egusphere-egu26-13669, 2026.

EGU26-14234 | PICO | TS1.2

Dissolution-Precipitation dominated deformation in (ultra)high-pressure serpentinites from the Zermatt-Saas Meta-Ophiolite 

Luiz F. G. Morales, Jesus Muñoz-Montecinos, Alberto Ceccato, Rüdiger Kilian, and Silvia Volante

Serpentinites are key components in subduction zones, acting as primary carriers of water into the deep Earth and critically influencing seismic behavior. Several studies suggest that fluid-saturated deformation in serpentinized subduction channels may control a variety of processes associated with Intermediate-depth seismicity (~50 to 300 km depth) . A key problem in their rheology is the discrepancy between experimentally deformed serpentinites, which exhibit predominantly brittle behavior, and their naturally deformed counterparts, which show ductile fabrics. While the dominant deformation mechanism in subduction settings—whether crystal plasticity, dissolution-precipitation, or a combination— also remains poorly documented. Moreover, there is a lack of constraints on how serpentinites deform during and after partial dehydration at (ultra)high-pressure conditions and transformation to olivine and pyroxene-dominated assemblages. To address these issues, we present an integrated microstructural and geochemical study of serpentinites across a hectometer-scale strain gradient within the Zermatt-Saas meta-ophiolite, documenting the evolution of deformation and major element mobility during subduction and exhumation. In low-strain samples, dehydration forms coarse-grained olivine-diopside-clinohumite-magnetite veins. Host antigorite shows weak crystallographic preferred orientations (CPOs) and twinning. With increasing strain, deformation localizes around these veins, where olivine develops a weak B-type CPO, but with grains showing no evidence of intracrystalline deformation. Progressively, antigorite develops a strong, penetrative foliation with a (001) maximum normal to foliation and grain size reduction, while olivine veins are folded and boudinaged. Low angle grain boundaries are related to fracturing of olivine. In high-strain serpentinite mylonites, transposed olivine veins form isoclinal folds, and S-C' fabrics develop. Antigorite CPO strength increases considerably, something that is not observed for olivine. Whole thin section XRF mapping reveals an increase of Ni and S in the more deformed serpentinites, where pentlandite defines the C' fabric and wraps around olivine porphyroclasts. Antigorite mm thick bands show Cr depletion accompanied by grain size reduction, while Fe-Mn occur normally associated with each other. In the transposed olivine veins there is an increase of Fe content in comparison to the original olivine vein composition.  When present, Al-rich phases such as chlorite are mostly undeformed but can breakdown locally and transform into tremolite + magnetite in late shear bands. Our data document a fluid-assisted progression from localized brittle-ductile to distributed ductile deformation. Microstructural and chemical evidence indicate that deformation was primarily controlled by dissolution-precipitation processes, with limited crystal plasticity in antigorite and predominantly brittle olivine deformation. This study provides a rare dataset on metamorphic olivine deformation in subduction zones and highlights the fundamental coupling between element mobility, metamorphic reactions, and strain localization in the subduction interface and mantle wedge.

How to cite: Morales, L. F. G., Muñoz-Montecinos, J., Ceccato, A., Kilian, R., and Volante, S.: Dissolution-Precipitation dominated deformation in (ultra)high-pressure serpentinites from the Zermatt-Saas Meta-Ophiolite, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14234, https://doi.org/10.5194/egusphere-egu26-14234, 2026.

EGU26-15191 | ECS | PICO | TS1.2

 Microstructure Across Deformation Regimes: 3D Imaging of Olivine by Dark-Field X-ray Microscopy 

Yaozhu Li, Phil McCaulsand, Roberta Flemming, Can Yildirim, and Carsten Detlefts

Olivine is a fundamental rock-forming mineral for which microstructures are closely tied to deformation conditions. However, visualization of olivine deformation has traditionally been limited to two-dimensional observations, ranging from petrographic microscopy at the millimetre– to micrometre scale to electron-based techniques probing crystallographic distortion and ordering at the micro- to nanometre scale (e.g., EBSD and TEM). Here, we introduce dark-field X-ray microscopy (DFXM) and present its first application to geological materials, conducted at beamline ID03 of the ESRF.

Using a focused line beam produced by compound refractive lenses, DFXM enables non- destructive, in-situ imaging with spatial resolution down to ~35 nm. By selectively illuminating a ~500 nm thick volume with the line beam, DFXM allows “slicing” through depth of the crystal volume. By translating the sample through the X-ray beam, the layers can be stacked and reconstructed into full 3D datasets.

In this work, we reconstruct the 3D microstructures of the mineral olivine across a range of deformation settings, spanning from hydrothermal single crystal olivine, to olivine in Åheim orogenic peridotite which experienced long-term dislocation creep, to olivine in heavily shock-metamorphosed martian basalt with relict crustal strain. We observe individual static dislocations and associated lattice strain field in the hydrothermal olivine single crystal, to arranged low-angle boundaries (LABs) formed by geometrically necessary dislocations (GNDs) in the Åheim peridotite, to chaotic dislocation networks connected by dense, short, and randomized LABs in shocked martian basalts.

By bridging conventional 2D crystallographic observations with volumetric 3D microstructural reconstructions, our work enables robust observations of microstructures developed in distinctive deformation conditions, providing a powerful and advanced 3D imaging technique for geological materials. Our study expands the application of DFXM to Earth and planetary materials and demonstrates the power of multi-scale, three-dimensional imaging for resolving complex deformation histories in geological systems.

How to cite: Li, Y., McCaulsand, P., Flemming, R., Yildirim, C., and Detlefts, C.:  Microstructure Across Deformation Regimes: 3D Imaging of Olivine by Dark-Field X-ray Microscopy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15191, https://doi.org/10.5194/egusphere-egu26-15191, 2026.

EGU26-15835 | PICO | TS1.2

Microanalytic characteristics of extremely fractured quartz in fault damage zone and implications 

Wen-Jie Wu, Po-ying Lien, Teng-Huei Huang, Wyan Chiu, Ching-Yu Chiang, and Li-Wei Kuo

The fault damage zone of the active Milun Fault in eastern Taiwan exhibits fractured and altered fault-rock textures, including spotted schist, serpentinite, and associated gouge. In the vicinity of the upper boundary of the damage zone, the recovered drill core hosts a non-cohesive, pulverized quartz body (~20-30 cm in length) within the fault rocks. The pulverized quartz is sandwiched between fractured schist and millimetre-scale laminae subparallel to the zone boundary. Microanalytical observations show that the quartz is shattered into a fine powder without an evident shear sense or preferred fracture orientation. No shear-induced amorphous phase is detected, whereas Laue diffraction indicates pronounced lattice distortion and elevated residual stress. The pulverized quartz displays a dense tensile fracture network, a feature commonly reported for seismically pulverized rocks along seismogenic faults, suggesting a dilatational, tensile-dominated fragmentation mechanism rather than progressive shear comminution. We propose that the quartz pulverization resulted from high strain rates associated with transient tensile stresses during coseismic rupture, potentially favoured by specific lithologic conditions.

How to cite: Wu, W.-J., Lien, P., Huang, T.-H., Chiu, W., Chiang, C.-Y., and Kuo, L.-W.: Microanalytic characteristics of extremely fractured quartz in fault damage zone and implications, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15835, https://doi.org/10.5194/egusphere-egu26-15835, 2026.

EGU26-16278 | ECS | PICO | TS1.2

Memory of brittle-ductile yielding within near surface fault zone sediments 

Jhardel Dasent, Ming Chang, Kenneth Su, Vashan Wright, and Michael Manga

The interactions between fluid and solids in fault zones are governed by slip, slip rate, and constituent properties. These interactions are recorded by particle shape and size distributions, fracture patterns, and the geochemical composition of material within the deformation zone. The evolution of near-surface sediment microstructures and yielding behaviors under tectonic loading and at variable fluid saturation remains an open question. We collect undisturbed 10 x 40 mm cores from unconsolidated silt-sized sediments (fines) surrounding, and along, a fault strand that slipped while saturated, and likely experienced aseismic slip under variable saturation over the past 300 years. We use X-ray microtomography to analyze voids within the fines and found that they are ellipsoidal, have volume distributions that are best fit by a truncated power-law, orient sub-parallel to the fault strike, and sometimes merge into tabular or irregularly shaped fractures. The volume range for power-law scaling in the distributions separates a smaller population of voids with markedly different distributions in sphericity, tortuosity, aspect ratio, and minor/major axis lengths from a larger population of voids. The power-law truncation is likely due to the finite core size. We interpret the voids as initially small gas bubbles that nucleated where cavities existed within the fines and then grew via diffusion of immiscible gases when saturated, or via brittle/ductile yielding of the fines under variable saturation. Several fractures cross-cut or branch off some voids, indicating multiple deformation events and suggesting that the void boundaries are weak spots within the fines that accommodate tectonic strain. Similar growth mechanisms have been observed in magmatic systems, where ductile yielding of the melt occurs from the merging of bubbles that primarily orient at acute angles from the maximum extension direction. These findings suggest that, in addition to sands, pore structures in finer-grained sediments preserve a record of near-surface aseismic slip and may provide a relative estimate of near-surface strain. The findings further imply that a process akin to ductile yielding deformed the fines and, in turn, the pore voids. 

How to cite: Dasent, J., Chang, M., Su, K., Wright, V., and Manga, M.: Memory of brittle-ductile yielding within near surface fault zone sediments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16278, https://doi.org/10.5194/egusphere-egu26-16278, 2026.

EGU26-17303 | PICO | TS1.2

Combined geochemical and textural analyses of halite: First results of non-destructive µXRF measurements 

Wilhelm Nikonow, Michael Mertineit, and Michael Schramm

The mineralogical-geochemical composition and texture of salt rocks plays an important role for the site selection and construction of a repository for heat-generating, highly active radioactive waste. As the bromide content in halite depends on the degree of evaporation and subsequent processes, Br is frequently analyzed to estimate the genetic history of the rocks (Braitsch 1971). Typically, geochemical analytical methods are applied on powder samples (e.g. ICP-OES, XRF), and textural analyses (e.g. using EBSD) require extensive sample preparation. In this study, first results of diapiric Upper Permian rock salt samples are presented using non-destructive µXRF on polished rock samples.

The µXRF Bruker M4 Tornado Plus (Nikonow & Rammlmair 2016) was used to map and quantify element distributions in rock salt. For calibration, in a first step, a certified reference material (CGL), consisting of mostly halite (NaCl) with minor content of anhydrite (CaSO4), and sylvite (KCl), was pressed into pellets of 2 g and 1 cm diameter. For representativity, three spot measurements and a mapping of the center (1 cm²) were chemically quantified. The µXRF measurements correlate with the certified values yielding an R² of 0.995. In a second step, pressed pellets with a range of defined concentrations of Br in halite and Rb in sylvite were prepared to estimate the concentration ranges measurable by µXRF. For Br, the concentrations range from 1 to 0.005 wt.% Br in halite, and for Rb the concentrations range from 0.4 to 0.005 wt.% Rb in sylvite. Both data sets show a good correlation with R² of 0.99 (n=21 for Br and n=17 for Rb). Therefore, µXRF seems suitable for quantification of Rb and Br in salt rocks.

Furthermore, naturally deformed halite samples were analyzed simultaneously for their geochemically and textural properties, which were previously analyzed using “conventional” methods (ICP-OES and EBSD, respectively; Mertineit et al. 2023). The bromide content in halite is ca. 200 µg/g and thus comparable to the known values. The textural results show misorientations of few degrees within single halite grains and pronounced misorientations at halite grain boundaries, indicating bending of the crystals, but no pronounced texture of the bulk rock.

Although the results are in good agreement with published data, further test should follow, especially on the textural analyses including the misorientation angle resolution and the indexing of the halite crystal axis. However, the application of µXRF on salt rocks offers a fast, non-destructive method providing reliable combined geochemical and textural information.

References

Braitsch 1971. Springer-Verlag, https://doi.org/10.1007/978-3-642-65083-3

Mertineit et al. 2023. Tectonophysics 847, https://doi.org/10.1016/j.tecto.2023.229703

Nikonow & Rammlmair. 2016. Spectrochim Acta B 125, https://doi.org/10.1016/j.sab.2016.09.018

How to cite: Nikonow, W., Mertineit, M., and Schramm, M.: Combined geochemical and textural analyses of halite: First results of non-destructive µXRF measurements, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17303, https://doi.org/10.5194/egusphere-egu26-17303, 2026.

EGU26-17416 | PICO | TS1.2

Advanced Microscopy and Machine Learning for Multiscale Analysis of Porosity and Mineralogy 

Joyce Schmatz, Mingze Jiang, and Julia Schmitz

Recent advances in microanalytical imaging and machine learning enable quantitative, multiscale characterization of geological materials with direct relevance for subsurface energy storage. This study presents an integrated workflow combining Broad Ion Beam (BIB) sample preparation, Scanning Electron Microscopy (SEM), Energy Dispersive X-ray Spectroscopy (EDX), and advanced machine learning to quantify pore structures, mineralogy, and their spatial relationships from the micrometre to nanometre scale (Klaver et al. 2021).

High-resolution secondary electron (SE2) and backscattered electron (BSE) imaging, complemented by low-resolution EDX data, provides multimodal datasets for automated analysis. Pore networks are segmented using a pre-trained U-Net deep learning model, enabling efficient and accurate porosity quantification. Mineralogical phases are identified and quantified through a semi-automatic, decision-tree–based segmentation approach. The alignment of SE2 and BSE datasets allows porosity to be directly correlated with specific mineral phases, establishing a robust link between microstructure, mineral composition, and petrophysical properties (Jiang et al, 2021).

The applicability of this technology-driven approach is demonstrated through two case studies. Case study 1 investigates geological hydrogen storage in underground salt caverns, focusing on the impact of biotic and abiotic reactions on anhydrite. Flow-cell experiments combined with cryogenic BIB-SEM analyses enable early detection of microstructural, mineralogical, and pore-space changes induced by hydrogen, hydrogen sulfide, and microbial sulfate reduction. Despite slow reaction kinetics, microstructural observations reveal the substantial onset of chemical alteration, biofilm formation, and evolving pore connectivity at the submicron scale, providing essential constraints for geochemical and hydraulic models (Berest et al., 2024).

Case study 2 examines fault sealing in mechanically layered limestone–marl successions. Oriented transfer samples from normal fault systems were analysed using multiscale microanalytical workflows to capture marl smearing, mechanical mixing, fracturing, and cementation processes. High-quality microstructural datasets serve as ground truth for training machine learning algorithms for efficient interpretation of 2D image data. The results show that fault cores are composed of recurrent structural building blocks whose distribution and sealing capacity are strongly controlled by the presence and properties of marly interbeds (Schmatz et al., 2022).

Overall, the integrated microscopy–machine learning framework provides a transferable, data-driven approach for quantifying coupled structural, hydraulic, and geochemical processes in complex geological systems.

References

Berest et al.,2024. Risk assessment of hydrogen storage in a conglomerate of salt caverns in the Netherlands. KEM-28 report. https://www.kemprogramma.nl/documenten/2024/04/03/kem-28-project-rapportfinal-report-kem-28-h2c3-240403_v2

Jiang et al., 2021.Workflow for high-resolution phase segmentation of cement clinker from combined BSE image and EDX spectral data. Journal of Microscopy, 1-7.

Klaver et al., 2021. Automated carbonate reservoir pore and fracture classification by multiscale imaging and deep learning. 82nd EAGE Annual Conference & Exhibition, Oct 2021, Volume 2021, p.1 – 5.

Schmatz et al., 2022. Prediction of Fault Rock Permeability With Deep Learning: Training Data from Transfer Samples of Fault Cores. 83rd EAGE Annual Conference & Exhibition, Jun 2022, Volume 2022, p.1 – 5.

 

How to cite: Schmatz, J., Jiang, M., and Schmitz, J.: Advanced Microscopy and Machine Learning for Multiscale Analysis of Porosity and Mineralogy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17416, https://doi.org/10.5194/egusphere-egu26-17416, 2026.

The investigation of microstructural characteristics in concrete constitutes a fundamental basis for advancing its performance in civil engineering construction. Existing expertise in digital rock physics (DRP), developed for natural rock materials, is transferred and adapted for concrete. DRP utilizes non-destructive X-ray computed tomography (XRCT) to examine the internal microstructure of concrete, allowing for the visualization of features such as phase distributions, pore space, and microcracks. In this study, high-resolution digital concrete twins are created to capture and quantify internal microstructural changes induced by external mechanical loading. To overcome limitations in phase and microstructure identification caused by the restricted resolution of XRCT, these digital investigations are complemented by detailed microstructural analyses using standard polarization microscopy and scanning electron microscopy (SEM). The results show that externally applied stresses significantly influence the microstructural response of concrete and thus affect the accuracy of physical measurements conducted under high-pressure conditions.

XRCT datasets with varying spatial resolutions were acquired under in-situ confining pressures ranging from 0.1 MPa to 46 MPa. CT images of concrete in unloaded and mechanically loaded states were subsequently analyzed and compared to identify stress-induced microstructural changes, with particular emphasis on the segmentation workflow. Here, particular focus is on large and small concrete aggregates, grain/phase boundaries within the aggregates, (micro-)porosity, and especially the interfacial transition zone (ITZ), which represents a major source of uncertainty in phase assignment during segmentation.

Image quality was first assessed by identifying artifacts and evaluating grayscale histograms. Subsequently, global thresholding was applied for phase assignment and initial segmentation, which was iteratively refined using complementary microscopic analyses of thin sections, including SEM, as reference data. The resulting segmentation of the concrete subvolume (600x600x769) distinguishes large and small aggregates (<80 % quartz, ca. 20 % phyllosilicates), pore space, phyllosilicate-composed matrix, silica-composed matrix, and inclusions (mainly rutile, zircon, apatite, iron oxides). Small changes can be seen in the distribution of the individual phases at the different pressures. With increasing pressure, the porosity decreases, and partially areas with characteristic phase arrangements arise along the large aggregates, potentially indicating the influence of the ITZ.

However, the quantitative determination of the interfacial transition zone remains challenging using XRCT data, and microcracks are likewise difficult to reliably resolve and segment. Therefore, the high-resolution microstructural investigations are also required to adequately capture these features. Overall, the study highlights the necessity of detailed microstructural characterization for the reliable interpretation of XRCT data and the assessment of stress-induced changes in concrete.

How to cite: Beiers, L. M., Balcewicz, M., Lebedev, M., and Saenger, E. H.: Digital Concrete Physics – Microstructural Characterization of Concrete under Confining Pressure: Insights from X-ray Computed Tomography and Microscopy , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17609, https://doi.org/10.5194/egusphere-egu26-17609, 2026.

EGU26-18276 | ECS | PICO | TS1.2

Deformation and reaction in the microstructural record of oceanic serpentinites 

Rebecca Kühn, Luisa Schlickum, Rüdiger Kilian, Luiz Morales, Andy Parsons, Barbara John, and Jeremy Deans

Ultramafic rocks exposed adjacent to mid-ocean ridges in the footwall to large slip oceanic detachment faults provide unique insight into deformation and reaction when transforming from peridotite to serpentinite. In contrast to orogenic serpentinites, oceanic serpentinites have not subjected to superposed metamorphic and/or tectonic overprinting. A suite of samples from mostly fresh peridotites (~20% alteration), with preserved olivine and pyroxene, to completely serpentinized rocks (100% alteration), dominated by serpentine (lizardite) and magnetite, were collected from a ~1.2 km long drill core from IODP Expedition 399 at the Atlantis Massif oceanic core complex.

A combined approach of synchrotron diffraction and electron backscatter diffraction in order to analyze the crystallographic preferred orientation (CPO), and micro X-ray fluorescence mapping and optical microscopy in order to image and analyze the microstructure, is used to explore the variable microstructures.

Magnetite forms polycrystalline aggregates defining a foliation, which ranges from anastomosing to highly parallel. In partially serpentinized, mylonitic peridotites showing olivine grain size reduction and CPO development; magnetite aggregates trace the preexisting mylonitic fabric. Lizardite and magnetite both have a variable CPO strength and different CPO types, suggesting that different processes and parameters influence the formation of these microstructures. Further, late stage deformation, is evident from microfaulting, sheared serpentine veins and dissolution features. The individual contributions of deformation and serpentinization reaction to the final microstructure will be evaluated and discussed.

How to cite: Kühn, R., Schlickum, L., Kilian, R., Morales, L., Parsons, A., John, B., and Deans, J.: Deformation and reaction in the microstructural record of oceanic serpentinites, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18276, https://doi.org/10.5194/egusphere-egu26-18276, 2026.

EGU26-18322 | PICO | TS1.2

Lithium content and mineralogical composition of fractured salt clay (Upper Permian) 

Michael Mertineit, Michael Schramm, Wilhelm Nikonow, and Jeannet Meima

Lithium is a trace component, which is frequently observed in salt deposits and salt solutions collected in salt mines, respectively (Mertineit & Schramm 2019). So far, no naturally formed Li-bearing salt mineral is known, thus, the origin of Li in salt deposits must be related to other sources, e.g. to detrital phyllosilicates (Braitsch 1971). Detailed investigations on the Li content, the occurrence within a mine and the mineralogical composition of specific stratigraphic layers enable the reconstruction of rock-fluid interaction and fluid migration pathways. This is important for the construction, design and dimensions for a repository for radioactive waste in rock salt.

To verify which minerals are Li-hosts, diapiric Upper Permian (Zechstein) samples from the uppermost Staßfurt-Formation and the lower Leine-Formation were investigated for their mineralogical-geochemical composition. The succession contains salt clays, anhydrite and carbonate rocks as these rocks reveal the highest Li content (up to 159 µg/g bulk rock). The samples were previously investigated using ICP-OES, ICP-MS, XRD, SEM and thin section microscopy. Beside typical salt minerals in varying amounts (halite, anhydrite, magnesite, sylvite, carnallite), most samples consist of quartz, illite-muscovite, chlorite (clinochlore) and biotite, all of them with a grain size of ≤100 µm, often <20 µm. Only few samples contain traces of kaolinite, koenenite, hydrotalcite, anatase and tourmaline.

Additionally, µXRF and imaging LIBS (Laser Induced Breakdown Spectroscopy) analyses were performed at the same specimen to obtain detailed information of the element distribution including Li on thick section scale (Nikonow et al. 2019).

The clay containing rocks are intensively deformed by boudinage and subsequent brittle fracturing. The fractures are oriented in different directions and are filled with halite and/or carnallite and single grains of anhydrite and magnesite. Relics of bedding are present, but the phyllosilicates do not show a pronounced shape-preferred orientation. Shear strain is indicated by a slight rotation of single rock fragments. The spatial distribution of Li shows that Li is enriched in certain areas. Li accumulations are observed in single silicate grains, which are unequally distributed in a very fine-grained clay matrix. Furthermore, Li is enriched at the fracture rims, often associated with seams of Fe-bearing phases and probably organic matter.

Depending on the mineralogical composition of the investigated rocks, the Li content varies significantly. Li probably originates from illite-muscovite and a Li-bearing variety of a tourmaline (elbaite). Li was mobilized during brine-host rock interaction and precipitated in fracture infill, probably at reducing geochemical conditions. However, due to the limited spatial resolution of most used methods compared to the very small grain size of the rocks, a distinct relation of Li content to a specific mineral phase requires further analysis.

 

Braitsch 1971. Springer-Verlag, https://doi.org/10.1007/978-3-642-65083-3

Mertineit & Schramm 2019. Minerals 9, 766; doi:10.3390/min9120766.

Nikonow et al. 2019. Mineralogy & Petrology 113, https://doi.org/10.1007/s00710-019-00657-z

How to cite: Mertineit, M., Schramm, M., Nikonow, W., and Meima, J.: Lithium content and mineralogical composition of fractured salt clay (Upper Permian), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18322, https://doi.org/10.5194/egusphere-egu26-18322, 2026.

EGU26-18619 | PICO | TS1.2

Recent Developments in 4D X-ray Tomography for Real-Time Observation of Fault Slip and Gouge Evolution 

Eranga Jayawickrama, Nick Harpers, Berit Schwichtenberg, Andrew Bell, Arthur Ng, Roberto Rizzi, Benoit Cordonnier, Marco Herwegh, and Florian Fusseis

The properties of fault slip surfaces, gouge characteristics, and fluid-rock reactions are tightly coupled and control earthquake mechanics. To visualise and quantify the role of this coupling, we have developed a new operando imaging approach that allows the documentation of fast direct-shear deformation experiments in time-resolved 2- and 3-dimensional image data at low single-digit micrometer resolution. A direct-shear inset developed for the X-ray transparent Heitt Mjölnir triaxial deformation apparatus enables experiments at 20 MPa normal stress under fluid-pressurised conditions and allows real-time permeability measurements.

We apply this platform to three fault systems: 1) Slip surfaces in basaltic rocks, imaged while sliding at 1 mm.s-1, reveal how asperities, phenocrysts, and surface roughness control stick-slip behavior and damage localization during fast slip. 2) Reactive quartz-gypsum gouges imaged during velocity stepping and healing experiments, enable the direct linking of evolving frictional properties to microphysical developments. 3) A shearing, dehydrating gypsum gouge provides insights into transient rheologies and the resulting strain distributions.

These datasets demonstrate that 4D imaging resolves coupled mechanical, chemical, and hydraulic fault evolution in real time. Our approach allows documenting microphysical processes underlying the frictional properties of faults and thereby constitutes a potent tool for studying faults in a variety of tectonic settings.

How to cite: Jayawickrama, E., Harpers, N., Schwichtenberg, B., Bell, A., Ng, A., Rizzi, R., Cordonnier, B., Herwegh, M., and Fusseis, F.: Recent Developments in 4D X-ray Tomography for Real-Time Observation of Fault Slip and Gouge Evolution, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18619, https://doi.org/10.5194/egusphere-egu26-18619, 2026.

The deformation and interaction of amphibole grains are crucial for comprehending the rheological behavior and physical properties of middle to lower crust. However, the mechanisms of strain accommodation and grain boundary processes in amphibolites are poorly studied. In this study, we analyzed a naturally deformed amphibolite from an exhumed continental strike-slip shear zone. The amphibole grains can be categorized into two distinct types: type I and type II, with the type II being embedded within type I. Type I amphibole grains exhibit typical plastic deformation behavior, distinguished by the presence of discernible dislocation arrays and formation of subgrains. In contrast, type II amphibole grains predominantly display microfractures in the middle of grains and voids occur in their elongated tails. Meanwhile, we identified three types of low-angle boundaries in amphibole grains with varying microstructural and nanoscale characteristics. Our findings indicate that low-angle boundaries in minerals are not exclusively associated with crystal-plastic deformation. Furthermore, the deformation characteristics in type II amphibole grains are related to grain boundary sliding (GBS) process. To relieve stress concentration during grain boundary sliding in type II amphibole grains, two accommodation mechanisms are proposed: (i) Grain boundary diffusion with elimination of grain boundary irregularities. (ii) Intragranular deformation of adjacent grains through either a brittle or a ductile process. Our findings hold significant implications for understanding the stress concentration and accommodation during deformation process in amphibolite

How to cite: Liu, J., Cao, S., and Cheng, X.: Development of low-angle boundaries in amphibole and their implications for accommodating grain boundary sliding in naturally deformed amphibolite, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20317, https://doi.org/10.5194/egusphere-egu26-20317, 2026.

EGU26-21052 | ECS | PICO | TS1.2

3D Fractal Analysis of Co-seismic Damage in the Nojima Fault Using X-Ray Tomography and SHPB Experiments 

Romain Iaquinta, Mai-Linh Doan, and Frederic Victor Donze

The origin of the intense damage found in active fault cores is still a matter of debate. We investigated the potential co-seismic contribution to this damage by studying the Nojima fault, which ruptured during the 1995 Kobe earthquake (Mw 6.9). Drilled just a year after the event, the Hirabayashi borehole offers a snapshot of the fault zone’s state shortly after a major rupture.

Working within the French ANR AlterAction, we analyzed drill core samples using X-ray computed tomography (CT) at a resolution of ~50 μm. Instead of relying on complex segmentation of fracture geometries, we applied a 3D fractal analysis to the spatial distribution of voids (empty space) versus the rock matrix. This method allowed us to quantify damage intensity and organization using the fractal dimension D. This metric, ranging from 2 (highly clustered voids) to 3 (homogeneous distribution), tracks the transition from localized fracture networks to diffuse pulverization and correlates well with fracture porosity.

We observed a damage zone extending roughly 70 m on either side of the fault core. While open fracture density generally spikes toward the core, it drops sharply in the immediate vicinity, likely due to rapid post-seismic healing. Our analysis shows D values near 2 in clustered zones, rising toward 3 where damage becomes volumetric. Interestingly, some samples display intense micro-fracturing but lack significant macroscopic deformation, resembling the "pulverized rock" seen at other active faults. This texture suggests high strain-rate loading occurred during the earthquake.

To test the dynamic origin of this damage, we ran Split Hopkinson Pressure Bar (SHPB) experiments on intact borehole samples to reproduce pulverization in the lab. We found a linear link between strain rate and absorbed energy. When combined with the CT data, this relationship helps distinguish two modes of propagation: diffuse pulverization (matching near-fault observations) and sparse, poorly connected networks. Crucially, the fractal dimensions of the experimental samples confirm these contrasting morphologies.

These results suggest that the intense damage in the Nojima fault core likely stems from co-seismic processes, marked by specific fractal patterns associated with high strain rates. We conclude that 3D fractal analysis of void space offers a robust tool, independent of geometry, for identifying the dynamic origins of fault zone damage.

How to cite: Iaquinta, R., Doan, M.-L., and Donze, F. V.: 3D Fractal Analysis of Co-seismic Damage in the Nojima Fault Using X-Ray Tomography and SHPB Experiments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21052, https://doi.org/10.5194/egusphere-egu26-21052, 2026.

EGU26-21418 | ECS | PICO | TS1.2

Probing active deformation - Fault healing through the lens of 4D operando imaging 

Berit Schwichtenberg, Florian Fusseis, Eranga Jayawickrama, Benoit Cordonnier, Nick Harpers, and Marco Herwegh

Direct observations of geological processes are often limited by available observation time, the spatial resolution of imaging techniques or the accessibility of active sites. These limitations also apply to fault healing, whereby faults progressively regain strength throughout the interseismic phase of the earthquake cycle. Here, conventional approaches either capture a static snapshot of the final microstructure in exhumed natural fault rocks or focus on the bulk mechanical behaviour through slide–hold–slide or direct shear experiments. However, these approaches generally fail to resolve the dynamic evolution of the microstructural record, and the associated chemo-mechanical feedback that controls a rock’s hydraulic properties. To overcome these limitations and constrain the spatiotemporal coupling between mechanical, chemical, and hydraulic processes in healing fault gouges, we conducted a series of direct shear experiments on analogue fault gouges composed of a quartz–hemihydrate mixture. We then monitored their microstructural evolution using operando 4D synchrotron-based X-ray CT imaging.

Our experiments, performed at constant shear rates of 0.3–1 µm/s, were designed to mimic gouge-rich faults in the uppermost continental crust during the interseismic phase. In the presence of a reactive pore fluid, we simulated chemical fault healing through dissolution-reprecipitation and cementation, which are associated with the hydration reaction of CaSO₄ hemihydrate to gypsum. In our deforming samples, these time-dependent healing processes compete with mechanical weakening processes, such as frictional granular flow.

Our novel approach combines an innovative experimental setup [1, 2] with high-resolution 4D imaging and advanced image analysis techniques, including digital volume correlation (DVC). In this contribution we discuss the benefits of integrating micromechanical data with high-resolution 4D imaging by linking active deformation mechanisms to the evolving mechanical and hydraulic response of the simulated fault gouge. Further, we demonstrate a shear-rate-dependent competition between time-dependent healing processes and mechanical weakening.   

 

[1] Freitas, D. et al. (2024): Heitt Mjölnir: a heated miniature triaxial apparatus for 4D synchrotron microtomography. Journal of Synchrotron Radiation 31, 150-161. doi.org/10.1107/S1600577523009876 

[2] Jayawickrama, E. et al. (2026): Recent Developments in 4D X-ray Tomography for Real-Time Observation of Fault Slip and Gouge Evolution, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18619.

How to cite: Schwichtenberg, B., Fusseis, F., Jayawickrama, E., Cordonnier, B., Harpers, N., and Herwegh, M.: Probing active deformation - Fault healing through the lens of 4D operando imaging, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21418, https://doi.org/10.5194/egusphere-egu26-21418, 2026.

Strike-slip faults critically control hydrocarbon migration in the Mesozoic clastic reservoirs of the Tahe Oilfield, NW China. However, their identification is challenged by weak seismic responses due to subtle impedance contrasts, steep dips, and small throws. This study conducts a systematic, multi-method comparison to optimize fault detection, evaluating both conventional seismic attributes and a novel deep learning (DL) approach.

We first applied structure-oriented filtering to enhance data continuity. Subsequently, key conventional attributes were computed: coherence and curvature to delineate major structural discontinuities and flexures, ant tracking to highlight fault pathways, and likelihood to map fault lineaments. The core of our DL approach involved a ResU-Net model, pre-trained on extensive datasets and refined via transfer learning using 65 manually interpreted fault traces from the target area. This process generated a high-resolution fault probability volume.

Results from the key T34 horizon demonstrate a clear performance hierarchy. While coherence and curvature effectively image major faults, they lack resolution for secondary networks. Ant tracking and likelihood show sensitivity to small-scale features but suffer from poor continuity and noise. In stark contrast, the AI probability volume integrates the strengths of these methods, simultaneously providing superior boundary clarity for major faults and enhanced detection of subtle, secondary strike-slip faults crucial for hydrocarbon migration. It presents a more continuous, spatially coherent, and geologically plausible 3D fault system.

This work underscores the significant advantage of an AI-driven, integrated workflow over individual conventional attributes. It provides a robust, scalable template for multi-scale fracture characterization in complex reservoirs, effectively bridging the gap between geophysical data analysis and geological interpretation.

How to cite: Jiang, Y. and Han, C.: Characterizing Mesozoic Strike-Slip Faults in China's Tahe Oilfield: A Multi-Method Comparison from Traditional Seismic Attributes to AI, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2170, https://doi.org/10.5194/egusphere-egu26-2170, 2026.

To clarify the migration characteristics of the X Sag trough in the Zhuyi depression of the Pearl River Mouth Basin and understand the distribution patterns of hydrocarbon source rocks, this study employs newly processed high-resolution 3D seismic data and integrates techniques such as fault activity period determination, fault displacement-distance curve analysis, and balanced section methods. It systematically investigates the deformation mechanism of the X Sag Fault in the Zhuyi Depression and its control over hydrocarbon source rock distribution. The study reveals: ① The X Sag is a north-dip, south-lobe scoop-shaped half-graben controlled by the NE-NEE-NWW multi-trend arc-shaped F1 fault, with three sets of secondary faults (NE, NEE, EW) developing within the depression. Based on the segmentation characteristics of the main boundary fault F1 and its combination patterns with secondary faults, the study area is divided into eastern and western sub-basins. ② The X Sag underwent multiple phases of tectonic evolution under the influence of multi-phase, multi-directional stress fields, primarily comprising four stages: Fracture Stage I, Fracture Stage II, Fracture Stage III, and the Tilting Stage. Based on the long-term activity characteristics of the main boundary fault F1 and the activity features of different phases of the secondary faults within the sag, five sets of fault systems were delineated: faults active only during the Early Wenchang Period, faults active during the Early Wenchang-Enping Period, faults active during the Late Wenchang-Enping Period, faults active only during the Enping Period, and long-term active faults. ③ The secondary faults within the X Sag are collectively controlled by a pre-existing arc-shaped NE-NEE-NWW-trending reverse-transform fault system. During basin formation, the western sub-sag underwent extensional deformation along pre-existing NE-NEE-trending faults, forming a series of secondary faults aligned with the main boundary fault strike. These appear in cross-section as structures reverse-cutting the main boundary fault. Conversely, the eastern sub-sag underwent extensional-torsional deformation along pre-existing NWW-trending strike-slip faults, generating a series of near-EW-trending secondary faults. During deformation, a “V”-shaped structural pattern formed in the profile. ④ The segmented growth and differential activity characteristics of different control-depression faults within the basin governed the migration of the depression trough sedimentary center from northwest to southeast and from the basin margin toward the basin interior, thereby influencing the distribution of hydrocarbon source rocks during the Early and Late Wenchang periods.

How to cite: Sun, X., Sun, Y., and Chen, F.: Deformation Mechanism and Its Depression Controlling-Source Controlling Effect of X Sag Fault System in Pearl River Mouth Basin, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2947, https://doi.org/10.5194/egusphere-egu26-2947, 2026.

Tectonic fractures refer to a series of discontinuities formed in crustal rocks under the action of tectonic stress, serving as a key factor governing numerous geological processes and resource exploitation. In the field of oil and gas exploration, especially for the tight sandstone reservoirs in the Kuqa Depression of the Tarim Basin, the tectonic fracture system acts as the primary seepage pathway and reservoir space, directly determining the distribution of reservoir "sweet spots" and single-well productivity. To achieve quantitative characterization of reservoir fractures and accurate prediction of their spatial distribution, we innovatively introduced the principle of minimum energy dissipation and the principle of least action, which reflect the essential laws of nature. By fully integrating the complex tectonic evolution process with classical mechanics theory, we completed the quantitative prediction research on fractures during complex tectonic evolution based on four-dimensional (4D) dynamic stress field simulation. Based on the analysis of tectonic evolution history in the Keshen 8 area of the Kuqa Depression, combined with extensive field, seismic, core and logging data, as well as rock mechanics experiments and acoustic emission experiments, a reasonable paleotectonic geomechanical model was established. From a novel perspective, we introduced the principle of minimum energy dissipation and the principle of least action, and further combined them with classical mechanics theory and the variational principle of continuum media. A time-domain dynamic rock failure criterion and a fracture parameter characterization model were constructed, building a "bridge" between stress and fracture parameters. By selecting an optimal elastoplastic finite element simulation platform and setting appropriate time steps, we completed the time-domain 4D tectonic stress field simulation. On this basis, we implanted Python programs into the finite element simulation platform, realizing the quantitative prediction of the spatial distribution of reservoir fractures in the Keshen 8 area of the Kuqa Depression. The prediction results indicate that folding is the primary controlling factor for fracture development in the Keshen 8 gas reservoir. On the plane view, the linear fracture density in the structural high parts of the east-west anticlines is slightly higher than that in the saddle parts and both limbs, and the linear fracture density in the core of the eastern anticline is higher than that of the western anticline. The fracture dip angle gradually decreases from the structural high points to the two limbs of the anticlines. The prediction results are in high agreement with the actual well-point measurement data and production performance data. High-yield wells are basically located in fracture-developed zones with high linear density and near-vertical dip angles.

How to cite: Liu, S., Wang, G., and Feng, J.: Quantitative Prediction of Tectonic Fractures Coupled with Minimum Energy Dissipation and Least Action Principles: A Case Study of Keshen 8 Area, Kuqa Depression, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3308, https://doi.org/10.5194/egusphere-egu26-3308, 2026.

EGU26-3360 | ECS | Posters on site | TS1.9

Effective fracture porosity in crystalline rock 

Josse van den Berg and Elco Luijendijk

Crystalline rocks are typically  low in porosity, but they often contain fractures, which provide critical pathways for fluid flow and influence groundwater storage, resource estimation, and safety assessments for nuclear waste repositories. Despite their importance, effective fracture porosity in crystalline rocks remains poorly constrained due to limited and regionally biased measurements. In this study, we used global permeability datasets and modified an existing equation to estimate porosity from permeability, incorporating fracture roughness and aperture. This allowed us to calculate nearly 28,000 porosity values across a wide range of depths and geological settings. The resulting porosity distributions are highly right-skewed and show an exponential decrease with depth. Our findings indicate that porosity values in crystalline rocks are generally lower than previously assumed. Median porosity values in the upper 100 meters are several orders of magnitude lower than the commonly assumed 1% porosity, highlighting a significant discrepancy between our estimates and traditional assumptions. We quantified uncertainty using Monte Carlo simulations, which show that natural variability in porosity dominates over parameter uncertainty, underscoring the robustness of our global trends. These findings imply that groundwater storage in crystalline rocks is far smaller than previously estimated, and groundwater velocities may be higher than predicted by models assuming larger porosity, with implications for contaminant transport and nuclear waste safety.

How to cite: van den Berg, J. and Luijendijk, E.: Effective fracture porosity in crystalline rock, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3360, https://doi.org/10.5194/egusphere-egu26-3360, 2026.

EGU26-3968 | ECS | Posters on site | TS1.9

New Integrated QDC-2D Toolbox for 2D Discontinuity Abundance Calculation 

Hrvoje Lukačić, Charlotte Wolff, Martin Krkač, and Michel Jaboyedoff

Quantitative characterisation of the geometrical properties of discontinuities in fractured rock masses is fundamental for understanding their mechanical behaviour, structural characterisation, and for performing reliable rockfall susceptibility assessments. Discontinuity abundance parameters, such as intensity and density, play a key role in rock mass classification and hazard analysis. Yet, accurately estimating them remains challenging due to limited accessibility, scale effects, and censoring bias in conventional field surveys.

Recent advances in remote sensing techniques, particularly UAV-based digital photogrammetry, enable the acquisition of high-resolution three-dimensional point clouds and ortho-view images, commonly referred to as Digital Outcrop Models (DOMs). These datasets significantly improve access to steep or unstable rock faces and enable detailed, reproducible discontinuity mapping. However, standardised, open-source tools for the quantitative analysis of discontinuity abundance from 2D ortho-view images remain limited.

Here, we present a new toolbox within the open-source MATLAB application QDC-2D (Quantitative Discontinuity Characterization, 2D) (Loiotine et al., 2021), focused on the calculation and spatial visualization of discontinuity abundance parameters. The toolbox computes commonly used linear (P10) and areal (P20, P21) discontinuity intensity and density metrics using two approaches. It uses well-established Mauldon estimators (Mauldon et al., 2001) and introduces a circular scan window approach that improves fracture intensity and density estimation through direct calculation of discontinuity trace segment lengths and number within the circular scan window. The toolbox further allows user-defined regions of interest (ROI) and cluster-based abundance calculation to capture spatial variability in discontinuity density and intensity. This approach enables the detection of high-fracturing zones with high certainty.

The toolbox's capabilities have been thoroughly tested and validated using multiple synthetic discontinuity datasets, demonstrating robust, reliable performance. This extension toolbox for QDC-2D provides a reproducible, accessible framework for quantitative discontinuity analysis, thereby supporting improved structural characterisation of fractured rock masses.

 

References:

Mauldon, M., Dunne, W. M., & Rohrbaugh, M. B., Jr. (2001). Circular scanlines and circular windows: New tools for characterizing the geometry of fracture traces. Journal of Structural Geology, 23(2–3), 247–258.

Loiotine, L., Wolff, C., Wyser, E., Andriani, G. F., Derron, M.-H., Jaboyedoff, M., & Parise, M. (2021). QDC-2D: A Semi-Automatic Tool for 2D Analysis of Discontinuities for Rock Mass Characterization. Remote Sensing13(24), 5086. https://doi.org/10.3390/rs13245086

 

How to cite: Lukačić, H., Wolff, C., Krkač, M., and Jaboyedoff, M.: New Integrated QDC-2D Toolbox for 2D Discontinuity Abundance Calculation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3968, https://doi.org/10.5194/egusphere-egu26-3968, 2026.

EGU26-4008 | Orals | TS1.9

Structural complexity and fault roughness properties of carbonate relay ramps 

Fabrizio Agosta, Stefania Dastoli, Carmela Taddeo, Ian Abdallah, Manuel Curzi, Marco Mercuri, and Amerigo Corradetti

The geometry and kinematics of small faults within relay ramps are affected by local stress perturbations due to coeval propagation of laterally overstepping normal faults with negligible separations. Independent of their stepping sense and relative fault slip rates, previous studies documented the high structural complexity of carbonate relay ramps cropping out in central Italy, where Mesozoic carbonates of the Lazio-Abruzzi Platform are crosscut by an active extensional fault system. Notably examples include the ~400 m-wide, ~900 m-long relay ramp within the Tre Monti fault dissected by small faults with variable attitudes and kinematics showing values of fault and fracture density peaks in its middle portion. Similarly, the ~3 km-wide, ~7km-long relay ramp bounded by the Venere-Gioia dei Marsi and Pescina-Parasano normal faults exhibits the highest amount of extensional strain within its central portion.

In order to gain new insights on the possible role of surface geometry of the main slipping planes on the spatial distribution of fault-related damage, we focus on the ca. 8 km-long, 110 m-offset, NW-SE striking and SW-dipping Monte Capo di Serre fault. This fault displaces Mesozoic-Tertiary platform carbonates and Pleistocene slope debris, and it is continuously exposed along a ~800 m-long along-strike outcrop. Studying a ~60 m-long and 32 m-wide relay ramp bounded by 100’s m- long fault segments forming a sinistral overstep, and at smaller scale a 9 m-long, 5 m-wide relay ramp bounded by 10’s of m-long dextral overstepping slip surfaces we first conduct field and digital structural analyses and then fault roughness analysis.

Results show that the slickenside attitude and kinematics are controlled by overstep geometry. In fact, dextral oversteps are associated with NNW-SSE to N-S striking high-angle slickensides recording pure-dip slip extension, whereas sinistral oversteps are characterized by ESE-WNW to E-W striking, moderate-angle slickensides recording left-lateral transtension. Independently of the overstep geometry, results of spectral analysis of the outcropping slickensides indicate they are significantly rougher (root mean square roughness, Rq≈25-68 mm) within relay ramps than along the main slip surfaces (Rq≈1 mm). Integration with microstructural observations suggests that the relay ramps localized diffuse post-seismic deformation and aftershock-related fracturing, as recorded by diffuse host rock brecciation and widespread fracturing. Conversely, the main slip surfaces predominantly accommodated seismic slip, as shown by truncated clasts and multiple generation of cataclasite and ultracataclasite layers. We argue that these results support the interpretation that fault-surface roughness within carbonate relay ramps might exert a primary control on local stress perturbations, thereby contribution to their complex structural and kinematics complexities.

How to cite: Agosta, F., Dastoli, S., Taddeo, C., Abdallah, I., Curzi, M., Mercuri, M., and Corradetti, A.: Structural complexity and fault roughness properties of carbonate relay ramps, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4008, https://doi.org/10.5194/egusphere-egu26-4008, 2026.

EGU26-4297 | ECS | Posters on site | TS1.9

Integrated field and laboratory analyses of vein assemblages from the downfaulted southern Apennines fold-and-thrust belt, Italy. 

Aji Kyari, Filippo Zummo, Ian Abdallah, Michele Paternoster, Antonio Caracausi, and Fabrizio Agosta

Along the downfaulted axial zone of the southern Apennines fold-and-thrust belt of Italy, ongoing work focuses on field survey of high-angle extensional fault zones, and integrated microstructural, mineralogical, and stable isotope analyses of fault-related calcite veins. Two study areas are investigated. The first one lies in the southern portion of the seismically active Irpinia region, the second one along the southern flanks of the Raparo Mt., Basilicata. There, we study Mesozoic shallow-water carbonates that first underwent thrusting tectonics, and then extension and exhumation from shallow crustal depths. Within the fault zones, we select the high-angle Slip Parallel veins (SP-veins) and low-angle Comb veins (C-veins), respectively oriented parallel and perpendicular to the fault dip.

In the Irpinia region, results of microstructural analysis of the vein assemblage indicate that the high-angle faults are characterized by veins containing blocky to elongated and fibrous calcite. Blocky calcite minerals show type I and II twinning. Furthermore, inclusion bands associated with crack-and-seal processes are also present. In line with established microstructural interpretations, blocky calcite is interpreted as post-kinematics, whereas elongated and fibrous calcite is regarded as syn-kinematics. Occurrence of type I and II calcite twinning suggests that the intracrystalline deformation temperatures in these regions falls within ca. 150o C - 300o C.

At the Raparo Mt., microstructural data are consistent with blocky, elongate-blocky calcite textures of both SP- and C-veins. The former veins are dominated by blocky calcite with established presence of Type I and II calcite twinning, while the latter veins occasionally show blocky calcite. This area also shows widespread occurrence of both high- and low-angle veins with microcrystalline textures, which suggest that rapid cooling of the mineralizing fluids and precipitation took place in their formation process. Common tar-rich mineralization is also observed along the low-angle veins.

Aiming at deciphering the relative timing of formation and paleo stress regimes, present work is dedicated to the detailed microscale documentation of the crosscutting/abutting relations among the different vein sets. At the same time, extraction of powder samples is taking place for subsequent geochemical analyses. Results will be key to determine the source/s of the mineralizing fluids, determination of isotopic fractionation, and amount of fluid-rock interaction. These analyses will enable formulation of valuable hypotheses regarding the modalities of ingression of the mineralizing fault fluids within the study fault zones.

How to cite: Kyari, A., Zummo, F., Abdallah, I., Paternoster, M., Caracausi, A., and Agosta, F.: Integrated field and laboratory analyses of vein assemblages from the downfaulted southern Apennines fold-and-thrust belt, Italy., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4297, https://doi.org/10.5194/egusphere-egu26-4297, 2026.

EGU26-4842 | Orals | TS1.9

Refining the picture of fracture development in folded carbonate reservoirs : Insights from U-Pb geochronology of syn-kinematic calcite mineralizations in the Provence fold-and-thrust belt, France  

Olivier Lacombe, Nicolas Beaudoin, Anies Zeboudj, Jean-Paul Callot, Juliette Lamarche, Guilhem Hoareau, Abel Guihou, and Pierre Deschamps

LA-ICP-MS U–Pb geochronology of syn-kinematic calcite in faults and fractures provides a direct means of dating brittle deformation. We present U–Pb calcite geochronological data from deformation features across a range of scales—stylolites, veins, minor faults, and major thrusts—within the Provence fold-and-thrust belt. Whether in thrust-related cover folds (Mirabeau and Bimont) or in the more complex Nerthe Massif, the results illustrate how calcite geochronology can enhance or challenge our understanding of fracture pattern development in reservoirs.

Calcite geochronology validates the sequence of fracture development during layer-parallel shortening, fold growth, and late-stage fold tightening, previously inferred from structural orientations and cross-cutting relationships, regardless of fold type. Dating of calcite jogs formed at the tips of sedimentary or tectonic stylolites further constrains the timing of deformation stages. Geochronology also helps differentiate local from regional deformation by defining a more precise chronological framework where other geological markers are absent.

Across all investigated structures, deformation features show remarkable age consistency and slight overlaps between stages, providing a continuous and detailed record of fracture development. The age overlaps may indicate that deformation lasted less than the analytical uncertainty or that fracturing was more continuous throughout folding and thrusting than previously assumed. The consistency of ages across structural scales suggests either coeval deformation or events too close in time to be distinguished by U–Pb dating. This observation supports the syn-kinematic nature of calcite mineralization in small tectonic veins, even where infills display blocky, non-stretched textures. While precipitation may lag slightly behind fracture opening in individual veins, at the vein-set scale, both processes remain coeval within dating resolution. This broadens the applicability of U–Pb calcite geochronology to diverse mesoscale structures.

The dataset reveals the multi-phase development of similarly oriented fractures, which possibly initiated during burial and were reopened or densified during subsequent tectonic episodes. Geochronology provides a robust way to test whether fractures grouped by orientation, deformation mode, and relative chronology (‘fracture sets’), as well as classical associations of veins, stylolites, and conjugate faults defined by kinematic and mechanical compatibility, truly reflect the same deformation event. Veins with up to 60° strike variation sometimes yield indistinguishable ages (within a few Myr), challenging conventional definitions of fracture sets and implying local stress variations. This questions the presumed stability of the stress field in tectonic reconstructions.

Regionally, clusters of U–Pb calcite ages, if not reflecting sampling bias, hint towards variations in fluid activity, redox conditions, and/or uranium mobility, or distinct pulses of brittle rock damage and fluid flow. The latter interpretation suggests two deformation phases—late Cretaceous (81–67 Ma) and late Paleocene–Eocene (59–34 Ma)—separated by a Paleocene tectonic quiescence, matching the two already recognized Pyrenean shortening phases and indicating a likely, though not systematic, link between regional tectonic activity, brittle rock damage, fluid circulation, and calcite mineralization.

These examples demonstrate how U–Pb calcite geochronology not only constrains the timing and duration of brittle deformation but also helps reassess models of fracture development and fold–fracture relationships.

How to cite: Lacombe, O., Beaudoin, N., Zeboudj, A., Callot, J.-P., Lamarche, J., Hoareau, G., Guihou, A., and Deschamps, P.: Refining the picture of fracture development in folded carbonate reservoirs : Insights from U-Pb geochronology of syn-kinematic calcite mineralizations in the Provence fold-and-thrust belt, France , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4842, https://doi.org/10.5194/egusphere-egu26-4842, 2026.

EGU26-5002 | ECS | Posters on site | TS1.9

Analysis of post-metamorphism brittle deformation in marbles: insights from Montagnola Senese, Northern Apennine 

Giacomo Risaliti, Roberto Emanuele Rizzo, Stefano Tavani, Massimo Coli, Jacopo Nesi, and Paola Vannucchi

The Tuscan marbles, primarily exposed in the Alpi Apuane Metamorphic Complex and the Montagnola Senese ridge, record a protracted deformation history spanning the rheological spectrum from ductile flow to brittle fracturing. While the syn-metamorphic ductile evolution of these units has been extensively studied, the subsequent brittle deformation—specifically post-metamorphic faulting and fracturing—remains poorly constrained. These fracture networks are not only uplift-related features; they record a polyphase brittle history with direct implications for fluid migration, quarry slope stability, and Neogene–Quaternary stress field reconstruction.

In this work, we characterize brittle structures within marble from the Montagnola Senese, located along the Mid-Tuscan Ridge in the Northern Apennines. This marble has been quarried since Roman times, making rock mass characterization relevant for both scientific and practical purposes. We adopt a multidisciplinary approach, integrating classical field surveys with 3D digital outcrop models obtained by photogrammetry. Data were collected at the outcrop scale and subsequently extrapolated to define the fracture pattern across the entire Montagnola Senese ridge.

The detected fractures and faults cut the marble schistosity, therefore post-dating the last metamorphism event (middle Miocene). Our results reveal at least two brittle deformation phases: (I) a first, left-lateral strike-slip system, followed by (II) extensional structures, which crosscut or reuse the previous ones. Fracture attributes, such as fracture intensity and density, within the non-faulted rock mass were compared to those associated with fault damage zones. These data provide constraints on both quarrying operations and fluid circulation models, whilst contributing to the definition of the tectonic setting of this sector of the Mid-Tuscan Ridge from the middle Miocene to the present day.

How to cite: Risaliti, G., Rizzo, R. E., Tavani, S., Coli, M., Nesi, J., and Vannucchi, P.: Analysis of post-metamorphism brittle deformation in marbles: insights from Montagnola Senese, Northern Apennine, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5002, https://doi.org/10.5194/egusphere-egu26-5002, 2026.

EGU26-5148 | ECS | Orals | TS1.9

Permeability Anisotropy in Fractured Mesozoic Platform Carbonates under Variable Triaxial Stress Conditions 

Ian Bala Abdallah, David Healy, Jeffrey Hyman, Giacomo Prosser, and Fabrizio Agosta

This study investigates how local stress state governs permeability magnitude in fractured carbonate aquifers. By using outcrop-constrained Discrete Fracture Network (DFN) modelling from Mt. Viggiano of the southern Apennines, Italy, we investigate the control exerted by 500 m-depth tri-axial local stress state on computed horizontal permeability anisotropy. Fractured carbonate systems commonly exhibit strong permeability anisotropies that evolve with depth as fractures respond to changes in both normal and shear stresses. Accurately capturing this behaviour remains challenging due to the combined effects of fracture geometry and connectivity, as well as primary depositional architecture and stress-dependent aperture modification.
Field-derived fracture datasets from four carbonate outcrops representing two contrasting paleo depositional settings are used to construct three-dimensional DFN models at the bed-package scale. Two DFN-based modelling workflows are employed to explore how different representations of fracture connectivity and flow influence predicted permeability. One approach estimates bulk permeability from fracture population statistics within distinct geocellular volumes. Differently, the other one explicitly simulates steady-state fluid flow through hydraulically connected fracture networks within a fully meshed computational domain. This integrated strategy allows evaluation of how modelling assumptions related to connectivity, aperture scaling, and flow representation affect permeability predictions without implying a preferred modelling tool.
The results of this study show that increasing normal stress generally reduces horizontal permeability anisotropy, although local increases in permeability occur where favourably oriented fractures undergo shear induced dilation. Result are also consistent with the permeability response varying systematically with depositional architectures: (i) massive, high-energy carbonates dominated by non-strata bound fractures exhibit vertically persistent but weakly connected networks; (ii) on the contrary, layered, low-energy carbonates containing abundant strata-bound fractures display enhanced lateral connectivity and higher hydraulic effective transmissivity.
The main outcomes of this work demonstrate that permeability anisotropy in fractured carbonates evolves with stress through its interaction with fracture orientation, connectivity, and stratigraphic architecture. Incorporating stress dependent behaviour and explicit connectivity into DFN workflows therefore improves predictions of subsurface fluid flow relevant to groundwater resources, CO₂ storage, and geothermal systems.

How to cite: Abdallah, I. B., Healy, D., Hyman, J., Prosser, G., and Agosta, F.: Permeability Anisotropy in Fractured Mesozoic Platform Carbonates under Variable Triaxial Stress Conditions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5148, https://doi.org/10.5194/egusphere-egu26-5148, 2026.

EGU26-5516 | ECS | Posters on site | TS1.9

Cracks in our foundations: The nature and origin of fissures in the Kortrijk Formation 

Loic Piret, Maarten Van Daele, Bruno Stuyts, Marc De Batist, Stijn Dewaele, Anis Kheffache, and Meghdad Payan

The stiff Ypresian clays of the Kortrijk Formation occur extensively throughout the subsurface of the Princess Elizabeth Zone (PEZ), North Sea. The formation is pervasively deformed with large-scale polygonal fault networks, so-called Clay Tectonic Features (CTF; e.g. Verschuren, 2019, Marine Geology). Moreover, recently acquired samples from the Kortrijk Formation in the PEZ suggest a heavily fissured internal structure of these clays at the centimeter scale. The presence of faults and fissures in this formation have strong implications for its geotechnical properties, such as strength and stiffness, which may pose challenges for the foundations of the planned offshore wind energy farms.

With this in mind, we study the physical, mineralogical and chemical properties of the Kortrijk Formation in high-resolution using a multi-methodological approach including X-ray CT scanning, organic and inorganic geochemical analyses (LOI, organic material, calcimetry, pH, stable carbon isotopes, pXRF, XRD and ICP-OES) and sedimentological investigations (grain size, thin sections). The first samples were collected from a 20m deep borehole with alternating rotary coring and hydraulic push sampling in Rumbeke (from a section that is considered stratigraphically equivalent to the PEZ) and multiple drilling campaigns at other locations are planned.

Initial X-Ray CT scans of these samples reveal a heterogenous internal architecture containing four main feature types: bioturbation, concretions, fissures, and faults. Bioturbation occurs throughout the cores, often appearing as millimeter-thick, centimeters-long, high-density features, likely reflecting the presence of precipitated minerals such as pyrite, following microbially-mediated sulfate reduction. In contrast, concretions (siderite-fluorapatite) are rare in the core sections, consistent with their observed scattered presence in land-based observations. Fissures are recognized as low CT-density features which do not occur throughout all the core sections but are concentrated in localized zones, leaving intervening volumes of clay intact. The observed cm-scale normal faulting structures point to a local extensional regime. The geometry, pattern, and textures of the observed fissures and fractures are tested against established criteria (e.g. radial and axisymmetry, bending near the core rim, etc.) to conclusively differentiate natural features from coring-induced artifacts (Adriaens et al., 2024, Geoenergy). To quantitatively analyze all features, the X-ray CT data are processed using a comprehensive workflow involving filtering, segmentation, and grouping of features based on multi-ROI analysis using 3D connectivity. Following isolation, we perform a detailed analysis of the morphological characteristics (e.g., volume, surface area) and the three-dimensional orientation of the segmented features. The high-resolution 3D model of the features in the clay derived from CT scanning will be used to inform numerical models which will test the stiffness and long-term mechanical stability of the Kortrijk formation clays under different geotechnical loading scenarios.

By combining detailed sedimentological, mineralogical and geochemical characterization with the high-resolution CT-based structural analysis, we aim to establish the origin of the fissures and faults in the Kortrijk formation, thereby providing the geological context for their impact on geotechnical stability.

How to cite: Piret, L., Van Daele, M., Stuyts, B., De Batist, M., Dewaele, S., Kheffache, A., and Payan, M.: Cracks in our foundations: The nature and origin of fissures in the Kortrijk Formation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5516, https://doi.org/10.5194/egusphere-egu26-5516, 2026.

The structural architecture of the Eastern Province of Saudi Arabia is defined by a complex interplay between localized halokinesis and regional compressional stresses. This study provides a comprehensive geological investigation into the mechanical and tectonic linkages between the heavily fractured Late Miocene-Pliocene Hofuf Formation and the Eocene Rus Formation situated at the apex of the Dammam Dome. Historically, these two units have been studied as distinct stratigraphic entities; however, this analysis integrates field observations from Jabal Al-Shuʿba with regional geophysical data to demonstrate a shared deformation history. The Dammam Dome, an oval-shaped structure covering approximately 500 km, is cored by the Infracambrian Hormuz Salt. Its diapiric rise, occurring at rates of up to 7.5 m/Ma during the Neogene, induced a systematic fracture network in the Rus Formation characterized by radial and concentric Mode I tension joints. Concurrently, the Arabian Plate's collision with Eurasia, the Zagros Orogeny, transmitted far-field intraplate stresses that reactivated these older structural grains. Field data from the Hofuf Formation at Jabal Al-Shuʿba reveal a high-intensity, multidirectional fracture system within alternating sandstone and mudstone beds. Unlike the uniform patterns observed at the Dammam Dome apex, the Hofuf fractures exhibit bimodal and conjugate orientations (NNE-NE and NW-SE) with apertures reaching 15 cm. This disparity is attributed to mechanical stratigraphy; the bed-bounded nature of fracturing in the clastic Hofuf Formation prevents the stress relief found in the massive Eocene carbonates, leading to increased fracture density. Furthermore, the identification of a soft-sediment detachment within the Rus Formation suggests that the Dammam Dome served as a sensitive stress sensor for the initial stages of the Zagros collision. By establishing a structural bridge between the Eocene and the Neogene, this study explains how salt-induced uplift and plate-scale compression have combined to create the heavily fractured landscape of Al-Ahsa. These findings offer critical insights for reservoir characterization, groundwater flow modeling, and urban geomechanical stability in the region.

How to cite: Osman, M.: Integrative Structural Evolution of the Eastern Arabian Platform: Decoupling Salt-induced Halokinesis and Zagros-related Compression in the Fractured Neogene and Paleogene Successions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5893, https://doi.org/10.5194/egusphere-egu26-5893, 2026.

EGU26-6648 | ECS | Posters on site | TS1.9

Implications of stress field evolution on groundwater flow at the northern Variscan front and its relevance for the Einstein Telescope site selection (Euregion Meuse-Rhine) 

Raphael Burchartz, Michal Kruszewski, Geert-Jan Vis, Hannes Claes, Alexander Müller, Yves VanBrabant, Jef Deckers, Philippe Orban, Daniel Drimmer, Mark Scheltens, Bjorn Vink, Michael Kiehn, Florian Amann, and Yvonne Spychala

The Einstein Telescope (ET), a proposed third-generation underground gravitational-waves observatory requires an acoustically quiet subsurface environment to minimize the effect of seismic ambient noise. A detailed site characterization is currently underway in the Euregion Meuse-Rhine (Germany, Belgium, Netherlands), one of the potential locations for the ET. The site is wedged between the northern margin of the Variscan deformation front and the subsiding Lower Rhine Graben. Subsurface fluid flow, including natural groundwater circulation and drainage constitute sources of induced seismic and gravity-gradient variations. Pre-existing faults and fractures act as preferential flow paths and, critically control potential water inflow into the infrastructure and influence related water management strategies. Consequently, characterizing the relationship between the tectonic stress field and hydraulic characteristics of the host-rock formations is essential for a resilient ET design. In this study, we investigate the evolution of the tectonic stress field (i.e., from paleo- to recent in-situ stresses) and its control on fracture permeability, using an integrated dataset of boreholes drilled in the study area from 2021 to 2025 and down to 250 to 420 m. Paleo-stress conditions are reconstructed from fracture orientations and kinematic indicators observed on drill core material and borehole-televiewer data. The present-day stress-state is evaluated using hydraulic fracturing and hydraulic testing of pre-existing fractures tests. Fracture architectures are characterized using televiewer imagery and core samples, while their hydraulic relevance is assessed through in-situ methods such as impeller flow-meter measurements, temperature logs, and hydraulic packer tests. Slip versus dilation tendency analysis is applied to evaluate deformation modes and associated permeability anisotropies. These results are compared to independent hydraulic indicators to distinguish between hydraulically active and inactive discontinuities. Our findings demonstrate how the complex tectonic history governs the present-day fracture network and associated groundwater pathways, providing key constraints on groundwater management and suitability assessments for the site selection of the ET project in naturally fractured sedimentary host-rocks.

How to cite: Burchartz, R., Kruszewski, M., Vis, G.-J., Claes, H., Müller, A., VanBrabant, Y., Deckers, J., Orban, P., Drimmer, D., Scheltens, M., Vink, B., Kiehn, M., Amann, F., and Spychala, Y.: Implications of stress field evolution on groundwater flow at the northern Variscan front and its relevance for the Einstein Telescope site selection (Euregion Meuse-Rhine), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6648, https://doi.org/10.5194/egusphere-egu26-6648, 2026.

EGU26-6896 | ECS | Posters on site | TS1.9

Investigating controls on exfoliation fracture geometry across glaciated and non-glaciated granitic domes, Yosemite National Park, USA 

Aislin N. Reynolds, Greg M. Stock, and Brian D. Collins

Exfoliation fractures are a defining feature of Yosemite’s granitic landscapes, yet the relative roles of lithology, glacial history, inherited structural fabrics, and near-surface thermal processes in controlling their geometry remain incompletely constrained. To evaluate these controls, we collected detailed field measurements across a suite of granitic domes spanning glaciated (Pothole Dome, Puppy Dome, Lembert Dome, Turtleback Dome, Olmsted Point) and non-glaciated (Half Dome, Sentinel Dome, North Dome) settings. Field investigations included systematic measurements of exfoliation sheet thickness and length, fracture orientation data, photographic documentation, and GPS surveys to assess spatial distributions of exfoliation fractures on individual domes. These data are integrated with lidar-derived topographic measurements to provide surface context and support geometry-based analyses.

Preliminary results indicate that exfoliation sheet thickness varies between domes, with glaciated domes tending to display thicker sheets and broader thickness distributions than non-glaciated domes, although substantial overlap exists between groups. Non-glaciated domes commonly exhibit thinner sheets and more variable geometries, potentially due to longer near-surface exposure and progressive weathering accumulation. Across all sites, exfoliation sheet length shows weak to moderate scaling with thickness; however, prevalent scatter in the data suggests that sheet geometry may not be influenced by thickness alone, but also by pre-existing joint sets and cross-cutting structural features that may limit lateral fracture propagation. Spatial context from GPS transects demonstrates that measurements were collected across broad surface positions on individual domes, with transects capturing tens to nearly 300 m of relief, reducing sampling bias and supporting dome-scale interpretation. Prior monitoring studies and field observations of rockfalls and active surface cracking in Yosemite suggest diurnal and seasonal thermal fluctuations contribute to ongoing subcritical crack growth, implicating thermal stresses as an active modern process superimposed onto background stresses (e.g., inherited structural features, removal of overburden, and tectonic and topographic stress). By comparing exfoliation characteristics across contrasting geomorphic settings, this study better constrains how factors such as lithology, glaciation history, inherited structures, and thermal forcing interact to shape near-surface fracture development in granitic terrains, with implications for rockfall hazard assessment and climate-sensitive rock damage processes.

How to cite: Reynolds, A. N., Stock, G. M., and Collins, B. D.: Investigating controls on exfoliation fracture geometry across glaciated and non-glaciated granitic domes, Yosemite National Park, USA, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6896, https://doi.org/10.5194/egusphere-egu26-6896, 2026.

EGU26-11582 | ECS | Posters on site | TS1.9

The role of pre-existing microcrack geometry in fracture initiation and propagation during elastic deformation: integrating LEFM analysis with FEM modeling 

Ludovico Manna, Matteo Maino, Leonardo Casini, and Marcin Dabrowski

Understanding the processes that govern fracture development in upper crustal rocks is crucial for characterizing the mechanical response of the Earth’s crust. While conventional failure criteria capture many aspects of fracturing observed in laboratory experiments, they fall short in explaining how system-spanning fractures emerge from the interaction and coalescence of microcracks distributed throughout a deforming rock mass. Additionally, empirical rupture models rarely distinguish the relative roles of tensile and shear mechanisms in macroscopic failure. In this study, we explore the influence of the geometrical arrangement of pre-existing microcracks on fracture formation by analyzing the elastic stress perturbations they generate, employing two-dimensional Finite Element Method (FEM) simulations. This approach allows us to quantify how cracks with different orientations modify the surrounding stress field, producing localized zones of elevated tensile and/or shear stress that may act as favorable pathways for fracture propagation. By systematically varying microcrack orientation and distribution, we can map how stress concentration patterns interact, providing a framework for understanding fracture coalescence in heterogeneous rock materials. Our results reveal that the orientation and spatial arrangement of pre-existing microcracks dictate the directions and magnitudes of stress perturbations, creating preferential trajectories for system-spanning fractures. In particular, regions of high tensile and shear stress develop between interacting cracks, offering a physical explanation for the formation of interconnected fracture networks, including en echelon fracture systems, under varying geometrical configurations. These findings indicate that macroscopic shear fractures may originate not only from the coalescence of tensile cracks formed during early deformation stages but also from the interaction of pre-existing cracks with different orientations, especially where tensile stress is concentrated at crack tips. The study demonstrates that the geometry of pre-existing microcracks is a primary factor controlling the spatial organization of resulting fracture networks. Fractures accommodating shear deformation, typically oriented at approximately ±30° to the axis of maximum compression, can arise from the coalescence of mode I cracks due to localized tensile stress concentration, rather than requiring shear-dominated initial conditions. This insight bridges a gap between classical fracture mechanics and observations of natural and experimental rock fracture systems, highlighting the interplay between tensile and shear mechanisms in shaping macroscopic failure patterns. Overall, our work emphasizes the importance of microstructural geometry in governing fracture evolution, offering a quantitative, framework which integrates LEFM analytical results with FEM-based models to predict the emergence of complex fracture networks from initial microcrack distributions. By linking local stress perturbations to large-scale fracture patterns, this study provides a more comprehensive understanding of the conditions leading to system-spanning fractures in the upper crust.

How to cite: Manna, L., Maino, M., Casini, L., and Dabrowski, M.: The role of pre-existing microcrack geometry in fracture initiation and propagation during elastic deformation: integrating LEFM analysis with FEM modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11582, https://doi.org/10.5194/egusphere-egu26-11582, 2026.

EGU26-12013 | ECS | Posters on site | TS1.9

Variability of Fault Damage Zone Width in Strike−Slip Faults: A Case Study from the Coast of Geoje Island, Korea 

Jinhyeon So, Yeoeun Seo, Kiwoong Park, Sangyeol Bae, and Young-Seog Kim

Fault damage zones are regions surrounding a fault core where secondary fractures are intensely developed due to distributed deformation. Previous studies on small-scale faults (consisting of one or two geometric segments) have predicted that the characteristics of the damage zone vary depending on the position along the fault. However, applying these models to large-scale fault zones is challenging due to the lack of continuous exposure and their inherent structural complexity.

This study aims to analyze the spatial variability of damage zone width in relation to fault geometry, focusing on medium-scale strike-slip faults (comprising three or more geometric segments), which offer a balance between structural complexity and observable continuity. The study area, Geoje Island, consists of hornfelsic Cretaceous lacustrine sedimentary rocks. The extensive wave-cut platforms along the coast provide excellent exposure for characterizing the geometry of the master fault and associated damage zones.

Fracture density (P21) was systematically quantified across fault segments and boundaries using circular scanlines arranged along strike-perpendicular traverses. The width of the damage zone along each traverse scanlines was determined by analyzing the changes in fracture density relative to the distance from the Principal Displacement Zone (PDZ). The results indicate that the width of the damage zone is highly variable and exhibits significant asymmetry in certain sections. Specifically, in linking damage zones, a widespread distribution of damage is observed beyond the extensional overlap zones, contrasting with patterns typically seen in small-scale faults. Furthermore, strong asymmetry is prominent in regions where the fault strike changes. However, such widespread damage distribution and asymmetry are well consistent with the characteristics of tip damage zones observed in small-scale faults.

These observations indicate that geometric complexity at these locations contributed to arresting rupture propagation during reactivation. Although individual rupture mechanics are similar across scales, the cumulative effect of geometric barriers in medium-scale faults appears to dictate the spatial evolution of the damage zone.  These findings are expected to provide valuable insights for predicting and understanding the architectural evolution of large-scale fault zones.

 

This research was supported by a grant (2022-MOIS62-001(RS-2022-ND640011)) of National Disaster Risk Analysis and Management Technology in Earthquake funded by Ministry of Interior and Safety (MOIS, Korea).

How to cite: So, J., Seo, Y., Park, K., Bae, S., and Kim, Y.-S.: Variability of Fault Damage Zone Width in Strike−Slip Faults: A Case Study from the Coast of Geoje Island, Korea, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12013, https://doi.org/10.5194/egusphere-egu26-12013, 2026.

EGU26-12608 | Posters on site | TS1.9

Syn-depositional fracture network prediction in carbonates through process-based forward modelling. 

Gerd Winterleitner, Sven Maerz, Nadezda Meier, and Jan Niederau

Early fracture networks in carbonate reservoirs may constitute long-lasting fluid flow conduits and their characterisation is pivotal in reservoir modelling. These fractures are, however, often overlooked in reservoir characterisation due to a lack of predictive workflows. Yet, syn-depositional fracture networks significantly affect reservoir quality and performance due to (1) providing an early and effective fluid flow network, (2) are prone to reactivation during later tectonic events and (3) are pathways for early dolomitising fluids.

Understanding the processes of fracture formation is vital for predicting their spatial distribution. Syn-depositional fracture modelling is, however, challenging as they form without tectonic drivers, influenced instead by intrinsic stresses due to the internal geometries of carbonate platforms. Early lithification of carbonates further aids fracture formation due to internal weaknesses and rapid sediment progradation. In reef-rimmed platforms, fractures generally align perpendicular to the platform’s trajectory, while internal patterns vary without a predominant orientation.

Traditional Discrete Fracture Network (DFN) models are inadequate for predicting these networks, as fractures result from complex geometries rather than regional stress fields. Process-based stratigraphic modelling offers a powerful workflow to model carbonate internal geometries and their lithofacies zones, linking progradation/aggradation patterns to fracture intensity and spacing.

We developed a novel approach for syn-depositional fracture characterization, combining stratigraphic and fracture forward modelling to improve reservoir quality predictions and well placements. Outcrop analogue studies are used for ground-truthing and to validate the findings against digital outcrop models. This innovative workflow has the potential to significantly improve flow performance assessment for carbonate geothermal reservoirs.

How to cite: Winterleitner, G., Maerz, S., Meier, N., and Niederau, J.: Syn-depositional fracture network prediction in carbonates through process-based forward modelling., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12608, https://doi.org/10.5194/egusphere-egu26-12608, 2026.

EGU26-13667 | ECS | Orals | TS1.9

Natural Fractures of the Tuscaloosa Marine Shale 

Cristina Mariana Ruse and Mehdi Mokhtari

The Tuscaloosa Marine Shale (TMS) is an unconventional play in southwestern Mississippi and southeastern Louisiana characterized by a well-developed network of natural fractures that strongly influences reservoir behavior and hydraulic fracturing performance. The play is significant to the energy industry due to its substantial hydrocarbon resources—estimated at approximately 1.5 billion barrels of oil and 4.6 TCF of gas—and its proximity to existing infrastructure. Although more than 80 wells have been hydraulically fractured in the formation, producing a total of 13.82 million barrels of oil and 9.04 BCF of gas, development remains challenging due to the shale’s high clay content, complex mineralogy, and the poorly constrained impact of natural fractures on production.

This study employs an integrated workflow to characterize natural fractures in the Tuscaloosa Marine Shale using electrical borehole image logs, shear-wave splitting data, and core descriptions from seven wells distributed across the play. The analysis indicates that the natural fractures are predominantly vertical to subvertical extension fractures, commonly fully mineralized, with heights ranging from 1 to 3 feet. These fractures preferentially trend east–west, are associated with calcite-rich intervals, and are capable of transecting the entire borehole. Smaller fractures often terminate at lithological boundaries but commonly reactivate along parallel planes.

The proposed methodology provides critical insight for optimizing hydraulic fracturing design by identifying stress orientation and optimal lateral placement relative to natural fracture distribution. In one lateral well alone, approximately 500 closed fractures were identified. Furthermore, the maximum horizontal stress orientation is shown to be consistent across the formation and aligned with the regional stress regime of the Gulf Coast Basin.

How to cite: Ruse, C. M. and Mokhtari, M.: Natural Fractures of the Tuscaloosa Marine Shale, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13667, https://doi.org/10.5194/egusphere-egu26-13667, 2026.

EGU26-13737 | Posters on site | TS1.9

NE-SW fault system in the eastern sector of the Trans-Mexican Volcanic Belt: Origin, deformation, and reactivation 

Alberto Vasquez Serrano, Elizabeth Rangel Granados, and José Luis Arce Saldaña

A NE-SW fault system described in the eastern sector of the Trans-Mexican Volcanic Belt (TMVB) has been active since the Pliocene and continued up to the Holocene with dip-slip kinematics. In a broad view, these NE-SW faults can be correlated to the Tenochtitlan fault system that extends from the southwest coast of Mexico to central Mexico, into the TMVB. The length of the faults, the damage zone width, and more than one slickensides on the fault planes suggests a complex deformation history. In this study, we investigate the geometry and kinematics of the NE-SW faults in the Miocene-Pleistocene rocks in the eastern sector of the TMVB to determine the kinematics of these faults during the Late Miocene to Holocene, for which it is unknown. Our results suggest that the Miocene rocks record two deformation events, one of which is related to crustal shortening that produced a strike-slip activity in the NE-SW faults during the Late Miocene. The second one is associated with crustal extension and the activity of the NE-SW faults with dip-slip kinematics. This extensional event was active during the Pliocene-Holocene. The reactivation analysis and our field observations suggest that the NE-SW normal faults are related to the reactivation of previous NE-SW strike-slip faults. The change in the kinematics of the NE-SW faults explains the complex geometry of the damage zones of the kilometric NE-SW faults and the highly fractured Miocene rocks.

Based on the fault system orientation, it is clear that these faults are incompatible with the field stress recorded in the eastern sector of the TMVB. This fact suggests that the NE-SW fault system is probably related to reactivated basement structures within a three-dimensional deformation with a complex deformation history. The activity type of the NE-SW faults is probably related to the dynamics of the subduction process in the southwest of Mexico, associated with the change in the dip (decrease) and the convergence velocity of the Cocos plate.

How to cite: Vasquez Serrano, A., Rangel Granados, E., and Arce Saldaña, J. L.: NE-SW fault system in the eastern sector of the Trans-Mexican Volcanic Belt: Origin, deformation, and reactivation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13737, https://doi.org/10.5194/egusphere-egu26-13737, 2026.

EGU26-14987 | ECS | Posters on site | TS1.9

Strike-slip fault zone architecture in folded Upper Malm limestones at Gorges de l’Orbe, Central Internal Jura, Switzerland 

Jefter Caldeira, Anindita Samsu, Ana Tanaka, and Loïc Bazalgette

Strike-slip fault zones often play a key role in controlling brittle deformation patterns in fold-and-thrust belts. Yet, the distribution of associated fractures and their interactions with fold-related structures remain insufficiently understood across scales and as part of the deformation history. In the Jura Mountains, previous work in the Central Internal Jura, notably at Creux-du-Van, proposed a multi-scale hierarchy of strike-slip faults and associated fracture networks based on sub-seismic structures spanning meter- to kilometer-scale. This study extends the multi-scale structural analysis to a regionally mappable ~12 km long N–S striking sinistral fault zone, the Suchet Fault. The fault is exposed along the E–W-oriented Gorges de l’Orbe, where incision into Upper Malm limestones enables largely continuous outcrop-scale access to fault-related damage zones.

To address the multi-scale character of this system, we combine field-based structural mapping at 1:5,000 scale and three-dimensional structural interpretation of publicly available aerial LiDAR data (SwissALTI3D) with systematic fracture data acquisition along four scanlines totaling 157 m. Scanlines are positioned at varying distances from the fault core, defined by the presence of fault breccia and gouge lenses, and across western and eastern structural compartments, spanning fault-proximal to fault-distal domains. This configuration enables comparison between fracture populations associated with fault-zone architecture and those interpreted as fold-related or background fracturing.

The Suchet Fault separates two contrasting structural domains. The western compartment is characterized by NW–SE striking fold trains, whereas the eastern compartment exhibits a comparatively flatter structural geometry. Within the vicinity of the fault trace, bedding orientations rotate progressively toward the N–S fault trend, with gentle eastward dips (~15°). Locally, near the fault core, bedding dips steepen and may reach up to 70°, indicating increased strain localization within the damage zone. LiDAR-based structural interpretation identifies three dominant fracture populations, with the NW–SE striking set displaying comparatively longer fractures than the N–S and NE–SW sets.

Fault-slip indicators show dominant subvertical conjugate strike-slip pairs at outcrop scale, comprising sinistral N–S to NNE-SSW striking faults and dextral NW–SE striking faults. Preliminary paleostress inversion analysis indicates a strike-slip regime characterized by a subhorizontal NW-directed maximum principal stress and a subvertical intermediate stress, consistent with results from other sectors of the Central Internal Jura. Fracture density (P10) increases toward the fault core, with values close to the brecciated core notably higher than those measured beyond 100 m.

This study emphasizes the need for robust fracture set definition and sequencing as a basis for structural analysis, including paleostress orientations and spatial variations in fracture intensity and anisotropy. This study evaluates whether structural patterns and paleostress behaviors identified at Creux-du-Van are comparable to those observed in the Gorges de l’Orbe area, at the scale of larger strike-slip fault zones. It also considers the potential regional implications of these structural features for fracture-controlled fluid flow in the Jura Mountains and potentially downstream, in the geothermal reservoirs beneath the Molasse Basin.

How to cite: Caldeira, J., Samsu, A., Tanaka, A., and Bazalgette, L.: Strike-slip fault zone architecture in folded Upper Malm limestones at Gorges de l’Orbe, Central Internal Jura, Switzerland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14987, https://doi.org/10.5194/egusphere-egu26-14987, 2026.

China hosts substantial lacustrine shale-oil resources and represents a key strategic replacement for sustaining reserves growth and production. Natural fractures are critical for enhancing the flow capacity of low-porosity, low-permeability, strongly heterogeneous lacustrine shale reservoirs and also exert fundamental controls on shale-oil accumulation and preservation. In the second member of the Funing Formation (E1f2) in the Qintong Sag, Subei Basin (eastern China), fractures are abundant and diverse, yet their development characteristics remain insufficiently constrained and a systematic evaluation of controlling factors has not been fully conducted. This study integrates core-based fracture description, thin-section petrography, and borehole image logs. Fractures are classified according to geological origin, mechanical mechanism, and geometric relationships with bedding, and their development characteristics are quantitatively documented. For multiple geological attributes—including distance to faults, mechanical layer thickness, TOC, and XRD-derived mineral contents—we employ Theil–Sen estimators to conduct a “score–confidence interval” ranking of effect strength and thereby delineate the hierarchy of controlling factors.Results indicate that bedding-parallel fractures, intra-layer shear fractures, and cross-layer shear fractures are dominant, whereas intra-layer tensile fractures and bedding-parallel shear fractures are subordinate. Fractures are predominantly high-angle, with apparent fracture height on core surfaces generally <15 cm. Fracture strikes comprise multiple sets, with a dominant NNE–SSW orientation. Fractures exhibit an overall moderate degree of infilling, and calcite is the principal cement. Distance to faults is negatively correlated with structural-fracture density and is identified as the primary control, whereas mechanical layer thickness and clay-mineral content are secondary factors and also show negative correlations with structural-fracture density. In contrast, higher TOC and greater lamination density promote the development of bedding-parallel fractures and constitute the primary controls, whereas higher clay-mineral content and greater mechanical layer thickness act as secondary factors that are unfavorable for bedding-parallel fracture development. These results clarify fracture distribution patterns in E1f2 and provide geological constraints for shale-oil exploration and development in eastern China, while also offering a transferable framework for the quantitative evaluation and ranking of fracture-controlling factors.

How to cite: Li, S., Lyu, W., Zeng, L., Shen, B., Ma, X., and Li, P.: Development characteristics and controlling factors of natural fractures in lacustrine shale oil reservoirs: A case study of the second member of the Funing Formation (E1f2), Qintong Sag, Subei Basin, eastern China, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15124, https://doi.org/10.5194/egusphere-egu26-15124, 2026.

EGU26-18303 | Posters on site | TS1.9

Anisotropy of fracture nodes using wavelet analysis 

Pradeep Gairola and Sandeep Bhatt

 Abstract:

Fracture networks play a critical role in controlling rock mechanics, fluid flow, and crustal deformation. However, many conventional analytical approaches do not adequately account for the spatial anisotropy of fracture nodes. This study introduces a wavelet-based angular variance method to quantify multiscale anisotropy in fracture network nodes, including I-, Y-, X-, and X + Y-nodes, as well as barycenters, using both synthetic and natural datasets.

Synthetic experiments demonstrate that isotropic fracture systems produce spatially random node distributions, whereas anisotropic systems generate distinct directional clustering, such as cross-shaped patterns aligned along NE–SW and NW–SE orientations. Application of the method to field data reveals strong correspondence between node anisotropy and underlying structural features. In the Jabal Akhdar dataset, X- and X + Y-nodes show pronounced elongation along an ENE–WSW direction, I-nodes exhibit weaker lobation in the same orientation, and barycenters remain largely isotropic. In contrast, the Getaberget dataset displays significant anisotropy across barycenters and multiple node types (Y, X, and X + Y), with dominant N–S to NNW trends consistent with NE–SW and NW–SE fracture sets.

These results demonstrate that wavelet-based node analysis is capable of detecting subtle, scale-dependent anisotropy in fracture systems. The proposed approach provides a sensitive, continuous, and scalable framework for quantifying fracture network organization, offering valuable insights for reservoir characterization, geothermal resource assessment, and the analysis of fracture-controlled fluid flow in geological systems.

 Keywords: Fracture network; Nodes; Spatial analysis; Point anisotropy; Wavelet analysis

 Acknowledgement

PG acknowledges the Indian Institute of Technology Roorkee and the Ministry of Human Resource Development (MHRD), Government of India, for support through a PhD fellowship. SB acknowledges financial support from the Department of Science and Technology (DST), Government of India (Project No: SRG/2021/001903), and from FIG (Grant No: FIG-100886-ESD), Indian Institute of Technology Roorkee, India.

How to cite: Gairola, P. and Bhatt, S.: Anisotropy of fracture nodes using wavelet analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18303, https://doi.org/10.5194/egusphere-egu26-18303, 2026.

EGU26-18351 | ECS | Posters on site | TS1.9

Indirect Rock Mass Characterization Using High-Resolution 3D Point Clouds Applied in Hazardous Rock Slopes 

Giampiero Mineo, Marco Rosone, Chiara Martinello, Claudio Mercurio, Edoardo Rotigliano, and Chiara Cappadonia

Rockfalls are among the most critical phenomena in geomechanics due to the significant risk they pose to human lives and infrastructure. Rockfall risk is defined by the interplay between hazard and the potential impact on exposed elements. Specifically, hazard assessment relies on the propensity for detachment (estimated frequency), event magnitude (volume), and intensity (kinetic energy).
Detachment propensity is governed by predisposing structural conditions and analyzed by the probability of failure modes, such as planar sliding, wedge sliding, or toppling, in relation to the main discontinuity sets. Conversely, magnitude and intensity depend on the probable volume of the unstable block and its potential propagation path.
Traditional geo-structural surveys, based on direct acquisition using standard instruments (e.g., geological compass and measuring tape), characterize, among other parameters, discontinuities in terms of orientation (dip angle/dip direction), spacing, and persistence. While the orientation of discontinuities, combined with mechanical properties, allows for the evaluation of the propensity to detachment, the definition of spacing and persistence is crucial for estimating block volume. However, this deterministic approach is often difficult to generalize to an entire slope, making accurate volume definition a persistent challenge.
To address this limitation and avoid the risks associated with direct data acquisition in hazardous areas, indirect remote sensing approaches have gained prominence. This study addresses the rockfall hazard characterization of a critical slope in the Palermo Mountain System (Sicily, southern Italy), where frequent rockfalls have disrupted vehicular traffic. Utilizing a Terrestrial Laser Scanner (TLS), the authors applied an indirect characterization method. Multitemporal acquisitions enabled a high-resolution 3D Point Cloud-based analysis, allowing for a more accurate and safe definition of hazard parameters in this complex environment.

How to cite: Mineo, G., Rosone, M., Martinello, C., Mercurio, C., Rotigliano, E., and Cappadonia, C.: Indirect Rock Mass Characterization Using High-Resolution 3D Point Clouds Applied in Hazardous Rock Slopes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18351, https://doi.org/10.5194/egusphere-egu26-18351, 2026.

EGU26-20377 | ECS | Posters on site | TS1.9

A multi-methodological workflow for fractured rock slope stability and block volume estimation  

Matteo Foletti, Niccolò Menegoni, Eugenio Poggi, Gianluca Benedetti, Massimo Comedini, Davide Elmo, and Matteo Maino

Fracture networks characterization is fundamental for assessing the stability of engineered slopes; although fractures are primary drivers of rock mass behavior, capturing their complexity across scales remains a significant challenge. This study presents a multidisciplinary workflow that integrates field-based geological interpretation with advanced remote sensing and numerical modeling to characterize fractured rock slopes. While recent progress in Remotely Piloted Aircraft Systems (RPAS) and Structure from Motion (SfM) has optimized 3D data acquisition, a gap persists in standardizing the transition from Digital Outcrop Models (DOMs) to representative geomechanical models, such as the rock block volume (Vb).

To bridge this gap, we propose an integrated workflow that compares and integrates results from field surveys, DOM and Discrete Fracture Networks (DFNs). By moving beyond traditional analyses (e.g., Markland Test and ISRM suggested approaches), which often oversimplify spatial complexity, our approach leverages high-resolution 3D data to improve the identification and prioritization of critical structural features. This framework was applied to the Molassana quarry (Genoa, Italy) as part of the SkyMetro project, demonstrating how us a multi-methodological workflow provides a more robust, data-driven assessment for large-scale engineered fracture slopes.

How to cite: Foletti, M., Menegoni, N., Poggi, E., Benedetti, G., Comedini, M., Elmo, D., and Maino, M.: A multi-methodological workflow for fractured rock slope stability and block volume estimation , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20377, https://doi.org/10.5194/egusphere-egu26-20377, 2026.

Successful pilot projects, e.g., CarbFix (Iceland) and Wallula (USA), where CO2 has been injected into subsurface basaltic rocks, have demonstrated the potential and advantages of mafic and ultramafic rocks (unconventional reservoirs) for long-term, safe CO2 storage by mineral trapping. Despite the advantages, the CO2 storage potential in unconventional reservoirs is relatively underexplored. Consequently, the key factors (and/or their interplay) that impact secondary mineralisation and the storage capacity of basaltic lava flows in the subsurface are less well understood. In this study, we integrate field-based geological investigation with whole-rock geochemical-, mineralogical-, and SEM- analysis, to characterise Miocene age Kaldakvísl basaltic lava flows, and associated deformation structures exposed along the western and eastern coastline of the Husavík–Tjörnes Peninsula, northern Iceland. Our results reveal at least two phases of fault activities and vein development in the western coast, associated with deformation along a major normal-dextral strike-slip fault, the Husavik-Flatey Fault Zone (HFFZ), whereas the eastern coast is far less deformed. Overall, the lava flows were largely characterized by tabular, sheet-like geometry, variable thicknesses ranging from c. 1 – 7 m, and sometimes interbedded with thin volcaniclastics and paleosols. Individual lava flows exhibited large variability in intra-flow vesicle morphology, intensity, connectivity, and mineral fill that allows us to subdivide each flow sequence into three distinct units: vesicular base-, massive core-, and vesicular top- of flow. Field observations and petrological analysis of lava flow sequences from the western coast show that the flow tops have been subjected to intense and higher degrees of hydrothermal alteration and secondary mineralization (e.g., zeolites and minor carbonates) compared to the flow base and core. Conversely, lava flow sequences from the eastern coast are generally less altered, preserving the primary composition and open vesicles of the lava flows. This suggests a strong correlation between the degree of deformation and tectonic fracturing, and the degree of hydrothermal alteration and secondary mineralization, underpinning the control the former has on the latter. Furthermore, the results of XRD analysis and optical microscopy identified zeolite minerals that formed both at lower temperatures (55-110 °C), such as chabazite and heulandite, and higher temperatures (70 °C up to 300 °C), such as stilbite and analcime. We propose that these zeolite minerals form from distinct hydrothermal events, reflecting a multi-stage rather than a continuous mineralization and alteration process. Our observations suggest that the multi-stage alteration process was most likely driven by the multiple phases of fault activities and vein formation associated with the HFFZ and subsidiary faults, which provided pathways for hydrothermal fluids. This study improves our understanding of the factors that influence hydrothermal alteration and secondary mineralization in basaltic rocks and has implications for evaluating the potential role of fractures in CO2 storage in unconventional reservoirs.

How to cite: Osagiede, E. E., Brechan, C. A., Bjørnsen, T. W., Nixon, C., and Rotevatn, A.: Fracture-controlled multi-stage secondary mineralization and alteration in Kaldakvísl basaltic lava group, Husavik–Tjörnes Peninsula, northern Iceland: implications for subsurface CO2 storage via carbon mineralization, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20981, https://doi.org/10.5194/egusphere-egu26-20981, 2026.

Shale oil reservoirs are typically characterized by ultra-low porosity and permeability, in which natural fractures provide key pathways for hydrocarbon migration from the matrix to the wellbore. These fractures significantly influence production performance. In the Mahu Sag of the Junggar Basin (NW China), the Permian Fengcheng Formation comprises saline lake–facies mixed shales with limited primary porosity, where natural fractures and dissolution pores dominate the available storage space. The sustained high single-well production (exceeding 100 t/day in parts of the sag) underscores the importance of understanding fracture occurrence and effectiveness for efficient reservoir development. In this study, we interpret Full-bore Micro-scanner Imager (FMI) borehole image logs using Schlumberger Techlog to identify and quantify both drilling-induced and natural fractures. The results show that drilling-induced fractures, which appear as short vertical features with symmetric “feather” or en-echelon patterns, are used to infer the orientation of the current maximum horizontal stress (SHmax). SHmax varies across structural domains: it trends near E–W to ENE–WSW adjacent to the Wuxia fault belt, shifts locally toward NE–SW at the junction of the Wuxia and Kebai fault belts, and transitions back to ENE–WSW to E–W toward the southwestern and southernmost regions. Natural fractures are abundant, predominantly striking NE–SW and near E–W (40°–100° and 220°–280°, accounting for 51% of fractures), with a secondary set trending NNW–SSE (140°–160° and 320°–350°, accounting for 22%). These orientations largely align with major fault trends. Fracture dip distributions vary significantly between wells and are primarily controlled by bedding attitude, with the apparent dip deflection closely mirroring the formation dip. In proximity to faults, tectonic fractures tend to exhibit lower dips. Aperture statistics reveal that fracture effectiveness is strongly stress-dependent: fractures more closely aligned with SHmax exhibit larger apertures and higher inferred effectiveness, while aperture size decreases with increasing misalignment angle. In a representative well, ENE–WSW fractures exhibit the largest mean apertures (tens of micrometers) compared to other fracture sets. Overall, SHmax) in the Fengcheng Formation shale is predominantly oriented E–W to ENE–WSW, and natural-fracture trends broadly match the strikes of major faults. Fracture dip angles are largely governed by bedding attitude, whereas fracture effectiveness is strongly stress-dependent. These results provide a direct basis for sweet-spot evaluation (targeting intervals with larger apertures under more favorable stress conditions) and for optimizing stimulation orientation and treatment design.

How to cite: Du, X. and Zeng, L.: Present-day stress control on natural fracture effectiveness: quantitative evidence from borehole image logs in the Fengcheng Formation shales, Mahu Sag, Junggar Basin, NW China, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21984, https://doi.org/10.5194/egusphere-egu26-21984, 2026.

EGU26-477 | ECS | Orals | TS3.2

Stress interactions in seismogenic faults through the lens of physics-based earthquake cycle simulations 

Constanza Rodriguez Piceda, Zoë Mildon, Billy Andrews, Jean-Paul Ampuero, Martijn van den Ende, Yifan Yin, Claudia Sgambato, and Francesco Visini

Recurrence intervals and magnitude distributions of earthquakes are key parameters in probabilistic and time-dependent seismic hazard assessments, yet they are difficult to constrain because the time window of instrumental and paleoseismic records often capture only a smaller fraction of the earthquake cycle of large earthquakes. Physics-based seismic cycle simulators can help to overcome these limitations by generating synthetic catalogues that span thousands of years, offering valuable insights into the statistical behaviour of fault networks. Despite the increasing use of these simulators, the physical mechanisms governing earthquake timing and size distributions remain incompletely understood, in particular the role of fault interactions and spatial variations in long-term slip rates.
Here we use the boundary-element code QDYN to simulate earthquake cycles on normal fault networks of increasing geological complexity, ranging from simplified two-fault configurations to realistic fault networks derived from field data in the Central and Southern Apennines (Italy). Our results show that both fault geometry and slip-rate variability critically influence earthquake recurrence and magnitude distributions. Networks with multiple across-strike interactions produce more complex seismic sequences, irregular recurrence intervals, and broader ranges of rupture sizes and moment magnitudes (Mw) compared to simpler configurations. Similarly, spatially variable slip-rate profiles promote diverse rupture behaviours, including partial ruptures and slow-slip events, that increase variability in stress redistribution, magnitude-frequency relationships and recurrence times. In contrast, models using uniform slip-rate profiles tend to produce regular recurrence patterns and characteristic earthquake magnitudes. These findings highlight the importance of incorporating realistic fault geometries and spatially variable slip rates in physics-based earthquake simulators used to inform seismic hazard assessments.

How to cite: Rodriguez Piceda, C., Mildon, Z., Andrews, B., Ampuero, J.-P., van den Ende, M., Yin, Y., Sgambato, C., and Visini, F.: Stress interactions in seismogenic faults through the lens of physics-based earthquake cycle simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-477, https://doi.org/10.5194/egusphere-egu26-477, 2026.

EGU26-1206 | ECS | Posters on site | TS3.2

Quantifying Off-Fault Plastic Strain in 3D Dynamic Rupture Models: Insights from the 2023 Kahramanmaraş Earthquake 

Rachel Preca Trapani, Yann Klinger, Mathilde Marchandon, Sébastien Hok, Oona Scotti, and Alice-Agnes Gabriel

The 2023 Turkey earthquake sequence generated widespread off-fault deformation. Recent 3D InSAR analyses of the doublet sequence show that ~35% of coseismic slip was accommodated by off-fault deformation extending up to 5 – 7 km from the fault (Liu et al., 2025). These observations, coined Absent Surface Displacement (ASD), may highlight the complex interplay between off-fault deformation, geometric fault complexity, and near-surface off-fault material properties. Quantifying how such deformation patterns emerge, and whether numerical earthquake models can capture their spatial organisation, remains an open question. 

In this study, we investigate the relationship between InSAR-derived ASD patterns from the MW 7.8 Kahramanmaraş rupture and synthetic off-fault plastic strain fields, which represent distributed inelastic yielding of the surrounding medium under dynamic rupture loading. This is generated in a suite of six different 3D dynamic rupture simulations with non-associative off-fault Drucker-Prager plasticity. These models extend on those presented in Gabriel et al. (2023) and incorporate varying on-fault frictional and structural complexities, such as fault roughness or fault waviness, variable fracture energy through different frictional parameters, and supershear initiation rupture speeds. We analyse fault-normal profiles along the geometrically complex rupture trace, and explore approaches for quantifying along-strike variability in inelastic yielding regions, plastic strain distribution and deformation asymmetry. Our analysis focuses on exploring whether off-fault plasticity can serve as a proxy for ASD and how geometric complexities and different dynamic rupture model ingredients influence the distribution and magnitude of off-fault deformation. This work provides an initial step toward constraining the consistency between observed and modelled near-fault deformation, and toward improving the representation of off-fault processes in physics-based earthquake rupture simulations.

How to cite: Preca Trapani, R., Klinger, Y., Marchandon, M., Hok, S., Scotti, O., and Gabriel, A.-A.: Quantifying Off-Fault Plastic Strain in 3D Dynamic Rupture Models: Insights from the 2023 Kahramanmaraş Earthquake, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1206, https://doi.org/10.5194/egusphere-egu26-1206, 2026.

EGU26-1323 | ECS | Posters on site | TS3.2

Postseismic evolution and megathrust re-coupling revealed by the spatio-temporal distribution of seismicity after the 2010 Maule earthquake 

Camila Monge, Marcos Moreno, and Valeria Becerra-Carreño

The 2010 Mw 8.8 Maule earthquake is one the largest and the best-instrumented megathrust ruptures worldwide, with extensive seismic and geodetic observations spanning its interseismic, coseismic, and postseismic phases, making it an exceptional case for understanding how a subduction interface relaxes and recouples after a great earthquake. In this study, we investigate the spatio-temporal evolution of seismicity with a focus on moderate-to-large seismic events (M ≥ 6) that occurred between 2010 and 2022 in the northern half of the Maule rupture and analyze how their deformation patterns reflect postseismic stress redistribution. While shallow aftershocks dominated the first two years following Maule, later seismicity concentrated around the margins of the main slip patch, where both afterslip and Coulomb stress changes were greatest. Only three M ≥ 6 earthquakes recorded in this interval generated measurable surface deformation: the 2012 Mw 7.1 Constitución, 2017 Mw 6.9 Valparaíso, and 2019 Mw 6.8 Pichilemu earthquakes. GNSS trajectory modeling combined with InSAR observations were used to characterize their coseismic deformation fields and invert for slip on the megathrust, revealing rupture patches consistent with independent constraints on Maule coupling and coseismic slip. The Constitución earthquake activated a deep asperity down-dip of the Maule high-slip zone, in a region that accumulated stress during early postseismic relaxation; the Valparaíso rupture occurred within a strongly coupled segment north of the Maule rupture that experienced enhanced loading and was preceded by a slow-slip episode; and the Pichilemu earthquake ruptured a shallow zone that underwent rapid afterslip before gradually re-locking. Together, these earthquakes demarcate a decade-long transition from afterslip-dominated deformation to the re-establishment of heterogeneous coupling along the megathrust, revealing that the Maule rupture continued to control regional tectonics long after the mainshock. These findings emphasize that moderate-magnitude events are key markers of ongoing stress redistribution and must be included to fully resolve the postseismic stage of the seismic cycle in one of the most active seismogenic subduction zones on Earth.

How to cite: Monge, C., Moreno, M., and Becerra-Carreño, V.: Postseismic evolution and megathrust re-coupling revealed by the spatio-temporal distribution of seismicity after the 2010 Maule earthquake, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1323, https://doi.org/10.5194/egusphere-egu26-1323, 2026.

EGU26-1374 | ECS | Posters on site | TS3.2

Limited near-trench slip of the 2025 Mw 8.7-8.8 Kamchatka earthquake from geodetic and tsunami data 

Chi-Hsien Tang, Yo Fukushima, Yutaro Okada, and Ayumu Mizutani

The Kamchatka subduction zone marks one of the most tectonically active regions in the world. Along the Kuril-Kamchatka Trench, the dense, cold Pacific plate subducts beneath the Okhotsk plate, accommodating a shortening rate of ~80 mm/yr along a direction almost perpendicular to the trench. Numerous tsunamigenic earthquakes have been documented along this subduction zone, including the 1952 Mw 8.8-9.0 megathrust earthquake that remains one of the largest events ever recorded by modern instruments. Similar megathrust events are suspected to have occurred in 1737 and 1841, although the observations from those times are scarce. On 29 July 2025, a Mw 8.7-8.8 earthquake occurred offshore Kamchatka, generating a tsunami that traveled across the Pacific. The 2025 epicenter lies less than 40 km from that of the 1952 earthquake and is accompanied by an aftershock distribution of comparable extent. The 2025 event therefore presents a rare opportunity to study the megathrust rupture on the Kamchatka plate interface using modern satellite-based geodesy.

We analyzed coseismic deformation of the 2025 Kamchatka earthquake using InSAR from multiple satellites and GNSS. InSAR images show deformation concentrated in the southern Kamchatka Peninsula, with amplitudes increasing progressively from inland areas toward the coast. The GNSS station on Paramushir Island recorded the maximum GNSS displacement, with seaward horizontal and downward vertical motions of ~1.7 m and ~0.2 m, respectively. Slip inversions suggest that the rupture propagated unilaterally from the epicenter to the southwest for ~480 km, broadly consistent with the aftershock distribution. The coseismic slip extended downdip to a depth of ~46 km, where the satellite-based geodetic data provide sufficient resolution. However, we found that inland geodetic measurements are insensitive to near-trench slip. Therefore, we generated three geodetic slip models with extreme, moderate, and zero shallow slip, and used DART tsunami observations to evaluate them. As a result, the model with zero shallow slip best reproduces the tsunami arrival times at DART stations, supporting the absence of significant near-trench rupture during the mainshock. The main rupture was confined to depths of 13-46 km, with a peak slip of ~9 m and a geodetic moment magnitude of Mw 8.7. The updip shallow portion of the 2025 rupture zone and the northern adjacent section may pose an elevated tsunami risk due to stress transfer. This work further underscores the crucial role of seafloor observations, as inland data typically offer limited insight into the shallow slip behavior of subduction interfaces.

How to cite: Tang, C.-H., Fukushima, Y., Okada, Y., and Mizutani, A.: Limited near-trench slip of the 2025 Mw 8.7-8.8 Kamchatka earthquake from geodetic and tsunami data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1374, https://doi.org/10.5194/egusphere-egu26-1374, 2026.

EGU26-1855 | Orals | TS3.2

Is long-term PSHA time-dependent? Insights from SimplETAS model 

Annamaria Pane, Francesco Visini, Simone Mancini, and Warner Marzocchi

Probabilistic seismic hazard analysis (PSHA) traditionally assumes time-invariant Poisson processes over mainshocks, while removing aftershocks through non-objective declustering procedures. This may underestimate seismic hazard, as recent sequences demonstrate significant ground-shaking contributions from aftershocks. Models for cluster correction (e.g., Marzocchi and Taroni, 2014; MT14) incorporate aftershock productivity but maintain temporally constant rates. While these models improve hazard estimates, the temporal persistence of conditioning effects in long-term forecasts remains poorly quantified.

This study investigates how long-term SimplETAS-based seismic hazard is affected by forecast initialization time, considering two scenarios: (i) an unconditional PSHA, i.e. not conditioned on a specific earthquake sequence, and (ii) a conditional PSHA initialized immediately after the 2009 L’Aquila earthquake sequence. We aim to assess whether 50-year PSHA remains consistent across different initialization times, which is typically assumed sufficient for the stationarity of the hazard process.

We employ the SimplETAS algorithm to generate two sets of 100,000 synthetic catalogs spanning 50 years: one set starting in 2024 (unconditional) and one starting immediately after the 2009 L’Aquila seismic sequence (conditional). For each earthquake in the synthetic catalogs, we assign a plausible seismogenic structure and compute fault-to-site distances for ground motion prediction using the GMPEs. Hazard curves are calculated empirically as the fraction of catalogs exceeding given PGA thresholds, without relying on the Poisson distribution. We analyze four Italian cities with varying seismicity levels: L’Aquila, Reggio Calabria, Firenze, and Milano. In the unconditional scenario, we compute 50-year hazard curves for all four cities. In the conditional scenario, we compute hazard curves for the same four cities to identify a conditioning effect only on the affected site of L’Aquila. Additionally, for that site, we quantify the temporal decay of conditioning by computing hazard curves over multiple time windows (1, 5, 10, and 50 years) and comparing them with the corresponding unconditional PSHA.

Unconditional PSHA shows good agreement with the reclustered version of the official Italian seismic hazard model (MPS19_cluster) across all four cities and different return periods, corroborating the use of SimplETAS-based approach for long-term PSHA, and the suitability of the MT14's PSHA correction across different return periods. The results of the conditional analysis reveal that L’Aquila exhibits differences of about 10-20% between conditional and unconditional PSHA even over the 50-year window, while Firenze, Milano, and Reggio Calabria remain essentially unchanged. The temporal decay analysis at L’Aquila shows how conditioning effects progressively decrease over longer periods, though the average effect remains detectable in a 50 years time window.

How to cite: Pane, A., Visini, F., Mancini, S., and Marzocchi, W.: Is long-term PSHA time-dependent? Insights from SimplETAS model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1855, https://doi.org/10.5194/egusphere-egu26-1855, 2026.

EGU26-2471 | ECS | Posters on site | TS3.2

Revisiting the early postseismic deformation of the 2003 Tokachi-oki earthquake 

Yuji Itoh, Cédric Twardzik, Mathilde Vergnolle, and Louise Maubant

A logarithmic function is the popular model of temporal evolution of afterslip, derived from the rate-and-state friction law (RSF) under the steady-state assumption (Marone+1991JGR). Relaxing this assumption, self-accelerating aseismic slip is predicted prior to subsequent decay even with velocity velocity-strengthening setting (i.e., a–b> 0; PerfettiniAmpuero2008JGR). The only natural observation example of such an accelerating stage of afterslip following large earthquakes is the case of the 2003 Tokachi-oki earthquake (M 8.0) in Japan, presented by Fukuda2009JGR (F09) with the data analysis performed by LarsonMiyazaki2008EPS (LM08). They reported that the early postseismic deformation emerged ~1 hour after the mainshock. We revisit this earthquake’s early postseismic deformation with a modern kinematic GNSS processing workflow by Gipsy-X v2.3 because many default and/or recommended settings and products have evolved from the time when these previous works were carried out. This revisit will align the Tokachi-oki case with other earthquake cases analyzed by GNSS processing strategies closer to ours than LM08’s.

Among all the parameters/settings of GNSS processing we tested, the most impactful parameter was the position random walk (RW) parameter. We tested a wide range of values from 1 to 1e-5 m/sqrt(s) for this parameter with switching to the white noise during the mainshock and the M 7.1 largest aftershock (1.3-h later). Comparing our test results with F09’s dataset, the largest mismatch was found between the mainshock and the 7.1 largest aftershock when we attempted to reproduce F09’s cumulative displacements. During this interevent window, F09’s dataset shows tiny deformation, while our solutions show significant deformation. On the other hand, our test solutions exhibit the acceleration at similar timings as F09’s, with the RW parameter same as F09’s (1e-5 m/sqrt(s)), but our cumulative displacements are much smaller than F09’s after the largest aftershock coseismic step was removed. This is because of a trade-off between early postseismic deformation and the largest aftershock step, caused by the very tight RW not allowing sites to move other than at the coseismic timing. Therefore, we recommend careful testing position RW parameter to accurately resolve early postseismic deformation, rather than taking a value introduced in other studies. With our test results, we concluded that no parameters could satisfactorily reproduce the early postseismic deformation presented in F09; in other words, the acceleration of early afterslip reported in F09 was absent in our solutions. Our results imply that the transition between the interseismic and postseismic stage of velocity strengthening faults would happen within several minutes at the longest, implying that the very beginning of afterslip is concurrent with the dynamic ruptures of the mainshock.

How to cite: Itoh, Y., Twardzik, C., Vergnolle, M., and Maubant, L.: Revisiting the early postseismic deformation of the 2003 Tokachi-oki earthquake, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2471, https://doi.org/10.5194/egusphere-egu26-2471, 2026.

Seismogenic depth is a fundamental parameter in seismic hazard assessment and is commonly inferred from kinematic approaches that rely on empirically defined thresholds. However, these observational estimates require validation and calibration against physics-based earthquake cycle models. Here we focus on the San Andreas Fault system in California, where high-quality geodetic, seismicity, and geothermal datasets are available. We construct a geodetically derived fault-coupling model for the entire fault system and systematically compare seismogenic depths inferred from fault coupling with those constrained by earthquake depth distributions. Our results show that a geodetic seismogenic depth defined by a coupling ratio of 0.45 provides the closest agreement with the depth enclosing 90% of the observed seismicity. This correspondence is quantitatively consistent with predictions from thermally constrained rate-and-state friction models, although the numerically inferred seismogenic depths are systematically shallower. Along-strike variations in seismogenic depth obtained from all approaches exhibit similar spatial patterns and correlate strongly with geothermal gradients, indicating that temperature is the primary controlling factor. These results establish a quantitative link between seismogenic depths derived from observational constraints and physics-based numerical models, thereby providing a stronger physical basis for incorporating geodetically inferred coupling models into seismic hazard assessments.

How to cite: Xu, X., Zhao, X., and Weng, H.: Discrepancies and controlling factors of rupture depths inffered from geodesy, seismicity and thermally constrained rate-and-state friction models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2700, https://doi.org/10.5194/egusphere-egu26-2700, 2026.

EGU26-3040 | ECS | Posters on site | TS3.2

Machine Learning for Liquefaction Hazard Mapping: A Case Study for New Zealand  

Denisa Tami, Roberto Gentile, Saurabh Prabhu, and Marco Carenzo

Earthquake-induced soil liquefaction poses significant risks to urban infrastructure in seismically active regions. Recent events, notably the 2011 Christchurch earthquake in New Zealand, demonstrate that liquefaction-induced damage can exceed that from ground shaking. This emphasises the need for scalable liquefaction hazard assessment tools. Traditional assessment methods that rely on cone penetration tests (CPT) and standard penetration tests are impractical for large-scale applications (e.g., regional hazard mapping or insurance portfolio analysis). This research develops a machine learning (ML) model that serves as a cost-effective proxy for traditional geotechnical testing.

Using CPT data from the New Zealand Geotechnical Database (NZGD), this study implements the state-of-practice Boulanger and Idriss (2016) methodology to calculate Liquefaction Potential Index (LPI) values for 5,879 unique locations across five Holocene geological units in New Zealand (i.e., windblown, human-made, estuary, river, and swamp deposits). ML models were trained separately for each geological unit to predict CPT-derived LPI, using three primary features: earthquake magnitude (Mw 5.0-8.0), peak ground acceleration (PGA) (0.05-1.2g), and groundwater table depth (0.5-15.0m). For each CPT location, the LPI was recomputed under sampled Mw-PGA-GWT combinations to create an expanded training set spanning plausible hazard and groundwater states. Using this training dataset, several ML methods were initially tested (i.e., gradient boosting, XGBoost, LightGBM, neural network, support vector machine), finally selecting LightGBM based on the best accuracy-training time trade-off. 

Model performance varied by geological unit: windblown deposits were captured well, achieving R2= 0.854, whereas river deposits reached only R2= 0.555, despite the latter having more training data. This finding demonstrates that depositional homogeneity, rather than data volume, can be more influential on ML performance in geotechnical applications. Feature importance analysis revealed balanced contributions to influencing predictions (i.e., magnitude: 33.7%, PGA: 34.5%, groundwater table depth: 31.8%), indicating the need to represent groundwater variability rather than treating shaking intensity as the sole dominant control. Validation against analytical LPI calculations for a synthetic scenario representing fully saturated conditions (Mw = 6.5, PGA = 0.4g, GWT = 0m) yields moderate agreement (R2= 0.491). The models tend to produce more conservative estimates for LPI < 5 and slightly underpredict for LPI > 40, likely reflecting systematic biases in the training data distribution, where extreme cases are underrepresented. Real-world application was also assessed by comparing predicted patterns with observed liquefaction manifestations during the 2011 Christchurch event from NZGD, independent of the training dataset. Comparisons observed good qualitative agreement with known high-susceptibility areas in eastern Christchurch, including zones near the Avon River and coastal margins. The proposed framework provides a scalable alternative to traditional CPT-based assessments, particularly for large-scale regional applications.

How to cite: Tami, D., Gentile, R., Prabhu, S., and Carenzo, M.: Machine Learning for Liquefaction Hazard Mapping: A Case Study for New Zealand , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3040, https://doi.org/10.5194/egusphere-egu26-3040, 2026.

Probabilistic Seismic Risk Analysis (PSRA) integrates seismic hazard with the vulnerability of exposed assets; however, the full propagation of uncertainties across this chain is still rarely examined. Although uncertainties affect hazard, vulnerability, and exposure models, most studies only partially address them, and end-to-end assessments remain limited. Epistemic uncertainty, arising from incomplete knowledge, is commonly represented through logic trees, which encode alternative modelling assumptions (e.g., recurrence models, maximum magnitudes) and define a discrete probability distribution over mutually exclusive options.

Previous studies suggest that hazard-related uncertainties often dominate seismic risk estimates, but few studies quantify this systematically, and is largely based on case studies from California. Within the TREAD project (tread-horizon.eu), we extend this understanding by applying a comprehensive framework to evaluate multiple sources of epistemic uncertainty using Italy, an earthquake-prone region, as both a national and regional case study.

We employ two alternative logic-tree structures: an area-source model with 540 branches and a combined fault-based plus smoothed-seismicity model with 243 branches. These configurations allow us to isolate the impact of choices related to slip rates, ground-motion models, scaling relations, recurrence behaviour, maximum-magnitude values, completeness methodologies, and site-specific assumptions.

Risk calculations are performed using the OpenQuake Engine, with structural economic losses adopted as the risk metric. Our results indicate that the dominant sources of epistemic uncertainty vary with the return period, implying that priorities for data acquisition and scientific investment should depend on the intended application of the risk results. Although ground-motion models often represent the largest contributor to epistemic uncertainty, our findings show that this assumption does not hold consistently across regions or return periods.

How to cite: Montejo, J., Silva, V., and Pace, B.: Influence of sources of epistemic uncertainties in hazard modeling on risk assessment: a regional assessment in Italy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3229, https://doi.org/10.5194/egusphere-egu26-3229, 2026.

EGU26-3242 | ECS | Orals | TS3.2

Scaling of Permeability Within Faults Across Nine Orders of Magnitude of Displacement  

Mohammadreza Akbariforouz, Qi Zhao, Chunmiao Zheng, and Daniel Faulkner

Faults are ubiquitous structures, ranging in length from millimeters to thousands of kilometers, with significant variations in permeability that regulate regional fluid flow, solute transport, seismicity, and hydrothermal circulation within the crust. Measurement of in situ fault permeability is challenging due to drilling difficulties and the risk of hydraulic fracturing. Moreover, existing scaling laws of laboratory permeability or fracturing intensity within faults are site-specific, highlighting the need for universal laws. Furthermore, damage zone permeabilities (kDZ) normalized to the protolith permeability (kNDZ) are typically high, while normalized fault core permeability (kNC) varies. We analyzed 752 in situ injection tests and 967 geomechanical experiments on seven faults with shear displacements (D) ranging from 1 to 5 m in the Asmari–Jahrum Formation (AJF), Iran. The AJF database was supplemented with 334 kDZ and 64 kNC datasets from the literature, covering 245 faults and spanning nine orders of magnitude in D. We quantified the hydraulic roles of fault cores as conduits (kNC>1) or barriers (kNC<1) based on porosity changes. We also developed kNC scaling laws using displacement divided by fault core thickness within a fuzzy-logic framework. A universal kNDZ law was established using distance from the fault core, damage zone thickness, and geomechanical parameters through kriging analysis. The universal material- and fault-dependent kNDZ and kNC laws indicate variations up to ten orders of magnitude in permeability. These findings enhance our understanding of fault hydrology and offer predictive tools for estimating fault permeability.

How to cite: Akbariforouz, M., Zhao, Q., Zheng, C., and Faulkner, D.: Scaling of Permeability Within Faults Across Nine Orders of Magnitude of Displacement , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3242, https://doi.org/10.5194/egusphere-egu26-3242, 2026.

EGU26-4289 | ECS | Orals | TS3.2

Exploring Fault Behaviour and Seismic Hazard in the Central Apennines through Earthquake Simulations 

Khatereh Saghatforoush, Bruno Pace, Alessandro Verdecchia, Francesco Visini, Octavi Gomez Novell, Olaf Zielke, and Laura Peruzza

The Central Apennines (Italy) are characterized by moderate seismicity and active fault systems capable of generating damaging earthquakes. However, the limited duration of historical and paleoseismic records restrict our understanding of long-term fault behaviour. In this study, we use the Multi-Cycle Earthquake Rupture Simulator (MCQsim) to construct a 3D model of 42 active normal faults and to generate multiple 100,000-year-long synthetic earthquake catalogues. We systematically vary key model parameters, including dynamic friction and fault strength heterogeneity, to assess their influence on earthquake occurrence rates, magnitudefrequency distributions, and rupture scaling.


The simulations reproduce the regional Gutenberg–Richter trend and show magnitude–average slip and magnitude–rupture area relationships consistent with empirical scaling laws and the available historical catalogue. Seismic productivity and rupture characteristics are most sensitive to variations in dynamic friction and fault heterogeneity. Although uncertainties arise from simplified fault geometries and assumptions about seismogenic depth, the overall agreement between synthetic and observed seismicity suggests that MCQsim effectively captures key aspects of long-term fault-system behaviour. These results indicate that physics-based synthetic earthquake catalogues can improve constraints on earthquake recurrence and rupture scenarios, providing valuable input for probabilistic seismic hazard assessment in regions characterized by moderate seismicity, complex active fault systems, and sparse observational data.

How to cite: Saghatforoush, K., Pace, B., Verdecchia, A., Visini, F., Novell, O. G., Zielke, O., and Peruzza, L.: Exploring Fault Behaviour and Seismic Hazard in the Central Apennines through Earthquake Simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4289, https://doi.org/10.5194/egusphere-egu26-4289, 2026.

EGU26-6377 | Posters on site | TS3.2

10Be-Based indentification of Paleoearthquake event on the Huashan Piedmont Fault 

Jinhui Yin, Wei Xu, Wenfang Shi, Jie Chen, and Marc Caffee

Over the past few decades, reconstructing paleoseismic sequences using in situ cosmogenic 36Cl exposure ages has proven effective in numerous countries and regions, greatly enhancing our quantitative understanding of active faults (Akçar et al., 2012; Benedetti et al., 2002; Goodall et al., 2021; Mitchell et al., 2001; Mouslopoulou et al., 2014). However, in China, where normal fault bedrock exposures are typically rich in quartz, 10Be is the optimal nuclide for dating fault scarps, offering a better fit to the local geological context than 36Cl. Despite this, only a handful of  10Be studies have reconstructed earthquake slip histories for large events (M>7) using the relationship between exposure ages and height on cumulative scarps (Lunina et al., 2020; Shen et al., 2016).
This study investigates the bedrock fault scarp at Duyu, situated along the Huashan Piedmont Fault (HPF)—the source of the AD 1556 M 8½ earthquake—using 10Be concentration profiling to identify paleoearthquake events. Our analysis confirms a strong earthquake occurred prior to the 1556 event, dated to 3092 ± 383 years ago. This finding bridges a significant gap in the paleoseismic record for this interval, which was previously undetected by traditional trenching methods. The HPF exhibits a quasi-periodic recurrence pattern with an estimated interval of 2623 ± 383 years. During the late Holocene, the fault maintained a vertical slip rate of 2.0 to 2.7 mm/yr, with individual events generating coseismic vertical displacements of 6 ± 0.5 m. These results demonstrate the value of in situ10Be exposure dating as a robust method for reconstructing the seismic histories of normal faults in tectonically similar regions globally.

How to cite: Yin, J., Xu, W., Shi, W., Chen, J., and Caffee, M.: 10Be-Based indentification of Paleoearthquake event on the Huashan Piedmont Fault, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6377, https://doi.org/10.5194/egusphere-egu26-6377, 2026.

EGU26-7786 | ECS | Orals | TS3.2

Direct marine geophysical constraints on the rupture of the 2012 Mw 8.6 Wharton basin earthquake 

Saksham Rohilla, Hélène Carton, Satish Singh, Muriel Laurencin, Nugroho Hananto, Mihai Roharik, Yanfang Qin, Sudipta Sarkar, Mark Noble, Mari Hamahashi, and Paul Tapponnier

Current understanding of earthquake rupture and earthquake cycles is largely derived from continental fault systems, implicitly assuming their applicability to oceanic lithosphere. Futhermore, the limited geological and geophysical constraints on large oceanic earthquakes hinder robust assessment of how deformation, fault growth, and stress accumulation takes place in the oceanic lithosphere. The 2012 Mw 8.6 Wharton Basin earthquake, the largest instrumentally recorded strike-slip event, challenged prevailing views of intraplate deformation in the Indian Ocean by rupturing a complex network of faults at high angles to one another. Seismological and geodetic analyses revealed a deep centroid depth, high stress drop, and multi-fault rupture, yet the offshore setting severely limited constraints on fault geometry and rupture propagation. Here, we bridge short- and long-term deformation processes by integrating high-resolution bathymetry, multichannel seismic reflection, and sub-bottom profiler data. We present the surface and near-surface deformation along one of the faults ruptured during the Mw 8.6 earthquake, which runs ESE-WNW and initiates near the epicenter of the Mw 8.2 aftershock. The ~100-km-long fault displays well-preserved dextral offsets accumulated since ~4 - 5 Ma and an en-echelon segmented pattern forming a positive flower structure rooted in the oceanic mantle. We estimate slip rates of ~0.4 to 0.8 mm/yr suggest long recurrence intervals for large intraplate earthquakes. Coulomb stress modelling indicates substantial coseismic stress loading on the N-S fault that subsequently ruptured during the Mw 8.2 earthquake, thus establishing a mechanical relationship between the two events. Overall, our study shows that the oceanic lithosphere can deform slowly and extensively over long time scales, accumulating strain along slow-slipping faults that can produce very large, cascade-style earthquakes. Furthermore, our study offers key inputs for earthquake cycle and dynamic rupture models in oceanic settings by providing geological constraints on fault geometry and slip rates.

How to cite: Rohilla, S., Carton, H., Singh, S., Laurencin, M., Hananto, N., Roharik, M., Qin, Y., Sarkar, S., Noble, M., Hamahashi, M., and Tapponnier, P.: Direct marine geophysical constraints on the rupture of the 2012 Mw 8.6 Wharton basin earthquake, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7786, https://doi.org/10.5194/egusphere-egu26-7786, 2026.

EGU26-8066 | Orals | TS3.2

Why closed seismic cycles matter for time-dependent seismic hazard: Lessons from global paleoearthquake records  

Vasiliki Mouslopoulou, Andy Nicol, Andy Howell, and Jon Griffin

The timing and size of the past large earthquakes that ruptured active faults are important to better understand seismic processes and time-dependent seismic hazards. A recent study highlights the rarity of ‘overdue’ earthquakes for New Zealand faults, a finding that directly contrasts observations from California, which indicate an unlikely long period of seismic quiescence. Here, we analyze paleoearthquake and historic records from 210 faults globally, including California, to test the international applicability of the findings for the New Zealand faults against a global active fault dataset. By comparing earthquake-elapsed and mean-recurrence data that derive from end-member fault systems, we explore the factors that control the shape of recurrence-interval distributions on different regions, and assess whether existing paleoearthquake and historical data can be used for estimating time-dependent seismic hazard. Our analysis: 1) demonstrates that the regions examined generally behave similarly for interevent and elapsed times, except for California which forms an outlier. This dissimilarity is important as faults in California have been commonly used to inform earthquake forecast models; 2) supports recurrence-interval distributions that are consistent with positively-skewed renewal models; and 3) proposes an improved approach for defining recurrence-interval distributions that involves the closed elapsed times constrained by historic ruptures and their penultimate events.

How to cite: Mouslopoulou, V., Nicol, A., Howell, A., and Griffin, J.: Why closed seismic cycles matter for time-dependent seismic hazard: Lessons from global paleoearthquake records , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8066, https://doi.org/10.5194/egusphere-egu26-8066, 2026.

EGU26-8422 | Orals | TS3.2

The anatomy of a strike-slip plate boundary fault in a pull-apart basin – The Motagua Fault in Guatemala 

Christoph Grützner, Tina Niemi, Omar Flores, Carlos Perez Arias, Aleigha Dollens, Jeremy Maurer, and Jonathan Obrist-Farner

Off-fault deformation in surface-rupturing earthquakes can be detected using geodetical methods, but field evidence is rare. Here we present data from the North American-Caribbean Plate boundary, documenting off-fault deformation in the geological record in great detail.

The Motagua Fault in Guatemala is part of the plate boundary between the North American and Caribbean plates. It ruptured in a M7.5 earthquake in 1976, producing a 230 km-long surface rupture with an average slip of about 1 m. At the Estanzuela site, the fault-parallel, elongated topographic depression “Laguneta Los Yajes” is about 2 m lower than its surroundings as revealed by new airborne LiDAR data. It is interpreted as a pull-apart basin, either caused by a fault stepover or by a fault bend. Since it was seasonally filled with water, the surface rupture of the 1976 Earthquake could not be mapped precisely here. We trenched the northern topographic scarp of the depression to investigate the boundary fault but did not encounter a distinct major shear zone. Instead, we found distributed deformation manifested as fractures. Two additional trenches in the center of the depression found the main fault zone and additional structures that accommodate distributed shear. We interpret the fault geometry to be a fault bend rather than a stepover, and we document the evidence for off-fault deformation over 80 m around the main strand at this site. These data shed light on the anatomy of the plate boundary and its associated off-fault deformation.

How to cite: Grützner, C., Niemi, T., Flores, O., Perez Arias, C., Dollens, A., Maurer, J., and Obrist-Farner, J.: The anatomy of a strike-slip plate boundary fault in a pull-apart basin – The Motagua Fault in Guatemala, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8422, https://doi.org/10.5194/egusphere-egu26-8422, 2026.

EGU26-8590 | ECS | Posters on site | TS3.2

Could Surface Precipitations Destabilize a Craton? 

Haibin Yang and Siyuan Zhao

The high integrated brittle strength of cratons with a cool and thick lithosphere protects cratonic interiors from tectonic deformation. High strain rates (>10-15 s-1) at plate boundaries facilitate enhanced faulting. However, cratons are not immuned from seismic activities. Intraplate earthquakes have caused more fatalities than interplate earthquakes. For example, the 1556 Huaxian earthquake (M 8.0), the deadliest earthquake in human history that killed 830,000 people, occurred in the middle of continental China. Seismic quiescent may in some stable continent relate to short instrumental histories (< ~150 years) with respect to the earthquake cycles (>104 years) and the limited resolution of geodetic surveys for fault motions in stable cratons. The extremely long earthquake cycles in stable continents make it hard to be detected due to surface erosional processes, particularly for those ‘one-off’ events. Classical seismic hazard estimation based on slip deficit calculations may not apply to earthquakes in stable continents when the last destructive earthquake occurred in history is unknown. To quantify the impact of seasonal hydrological cycles on seismicity in stable cratons, we integrate seismic catalogs with GRACE(-FO) data, borehole water levels, precipitation records, and InSAR observations from the Pilbara and Yilgarn cratons in Australia. Our analysis tests whether seismic responses to hydrological stress are consistent across cratons and assesses whether these perturbations induce temporary or permanent changes in craton stability.

How to cite: Yang, H. and Zhao, S.: Could Surface Precipitations Destabilize a Craton?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8590, https://doi.org/10.5194/egusphere-egu26-8590, 2026.

EGU26-10254 | ECS | Posters on site | TS3.2

Formation of Fault Damage Zones in Carbonates and Their Role in the Seismic Cycle 

Daniel Dreier, Mathilde Marchandon, Michele Fondriest, Alice-Agnes Gabriel, and Giulio Di Toro

Probably the most impressive geological feature of active fault zones hosted in carbonate rocks is the presence of several hundreds of meters thick damage zones, often composed of in-situ shattered rocks (ISRs, i.e. rocks fragmented into clasts < 1 cm in size). Despite their abundance, it remains unknown how ISRs form (during the propagation of seismic ruptures?), and how their presence affects (1) the propagation of individual mainshock seismic ruptures, (2) the near field wave radiation and associated strong ground motions, and (3) the evolution in space and time of aftershock seismic sequences. In this contribution, we will present preliminary results of a three-year Ph.D. project aimed at addressing these issues through an integrated field geology and numerical modelling approach.

We exploit existing and newly acquired field geology data on fault damage zone distributions in the Central Apennines (Italy), and perform dynamic rupture earthquake sequence simulations with SeisSol (https://seissol.org). The fully-dynamic individual earthquake simulations with SeisSol rely on the discontinuous Galerkin method, which allows treating complex 3D geological structures, nonlinear rheologies (including off-fault plastic yielding) and high-order accurate propagation of seismic waves (Käser et al., 2010). The earthquake modelling simulations integrate laboratory-derived frictional constitutive laws with simplified and realistic representations of fault zone geometry and surface topography. Currently, our study is focused on the 25 km long Campo Imperatore fault system in the Gran Sasso Massif area (Italian Central Apennines) where the damage zones are pronounced and well mapped (Demurtas et al., 2016; Fondriest et al., 2020).

We aim at using the dynamic rupture earthquake modelling simulations to discuss the formation and distribution of ISRs with respect to (1) the maximum magnitude (Mw 7.0) of the earthquake associated with the studied fault, (2) fault geometry (length, presence of step overs, fault bends, etc.), (3) topographic effects (valleys, etc.), and (4) lithology (limestones, dolostones, etc.) of the wall rocks. This approach is expected to identify the physical, geological, and loading conditions controlling seismic rupture propagation and the development of fault damage zones. The physically based, fully dynamic 3D simulations will also provide estimates of earthquake source parameters (e.g., fracture energy and seismic moment release rate) and synthetic seismograms (strong ground motions), which will be compared with seismological and strong-motion data from earthquakes in the Central Apennines.

 

References

 

Demurtas, M., Fondriest, M., Balsamo, F., Clemenzi, L., Storti, F., Bistacchi, A., & Di Toro, G. (2016). Structure of a normal seismogenic fault zone in carbonates: The Vado di Corno Fault, Campo Imperatore, Central Apennines (Italy). Journal of Structural Geology, 90, 185–206. https://doi.org/10.1016/j.jsg.2016.08.004

Fondriest, M., Balsamo, F., Bistacchi, A., Clemenzi, L., Demurtas, M., Storti, F., & Di Toro, G. (2020). Structural Complexity and Mechanics of a Shallow Crustal Seismogenic Source (Vado di Corno Fault Zone, Italy). Journal of Geophysical Research: Solid Earth, 125(9), e2019JB018926. https://doi.org/10.1029/2019JB018926

Käser, M., Castro, C., Hermann, V., & Pelties, C. (2010). SeisSol – A Software for Seismic Wave Propagation Simulations. In High Performance Computing in Science and Engineering, Garching/Munich 2009 (pp. 281–292). Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-13872-0_24

How to cite: Dreier, D., Marchandon, M., Fondriest, M., Gabriel, A.-A., and Di Toro, G.: Formation of Fault Damage Zones in Carbonates and Their Role in the Seismic Cycle, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10254, https://doi.org/10.5194/egusphere-egu26-10254, 2026.

EGU26-10477 | Orals | TS3.2

Seismic gap breached by the 2025 Mw 7.7 Mandalay (Myanmar) earthquake 

P. Martin Mai, Sigurjón Jónsson, Bo Li, Cahli Suhendi, Jihong Liu, Duo Li, Arthur Delorme, and Yann Klinger

Seismic gaps are fault sections that have not hosted a large earthquake for a long time compared to neighbouring segments, making them likely sites for future large events. The 2025 Mw 7.7 Mandalay (Myanmar) earthquake, on the central section of the Sagaing Fault, ruptured through a known seismic gap and ~160 km beyond it, resulting in an exceptionally long rupture of ~460 km. Here we investigate the rupture process of this event and the factors that enabled it to breach the seismic gap by integrating satellite synthetic aperture radar observations, seismic waveform back-projection, Bayesian finite-fault inversion and dynamic rupture simulations. We identify a two-stage earthquake rupture comprising initial bilateral subshear propagation for ~20 s followed by unilateral supershear rupture for ~70 s. Simulation-based sensitivity tests suggest that the seismic gap boundary was not a strong mechanical barrier in terms of frictional strength, and that nucleation of the earthquake far from the gap boundary, rather than its supershear speed, allowed the rupture to outgrow the gap and propagate far beyond it. Hence, we conclude that the dimension of seismic gaps may not reflect the magnitude of future earthquakes. Instead, ruptures may cascade through multiple fault sections to generate larger and potentially more damaging events.

How to cite: Mai, P. M., Jónsson, S., Li, B., Suhendi, C., Liu, J., Li, D., Delorme, A., and Klinger, Y.: Seismic gap breached by the 2025 Mw 7.7 Mandalay (Myanmar) earthquake, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10477, https://doi.org/10.5194/egusphere-egu26-10477, 2026.

EGU26-10546 | ECS | Orals | TS3.2

Three-dimensional anisotropy of seismite deformation constrains seismogenic fault location 

Xiao Yang, Xuhua Shi, Haibin Yang, Yann Klinger, Hanlin Chen, Jin Ge, Feng Li, Xin Liu, Yixi Yan, and Zhuona Bai

Earthquake ground motion is inherently directional and governs deformation in near-surface sediments, yet whether this directional information is preserved in geological archives remains poorly constrained. Soft-sediment deformation structures produced by earthquakes (seismites) are widely used to reconstruct past earthquake catalogues but are generally assumed to lack information on seismic-wave direction, limiting their ability to identify seismogenic faults. Here we develop a three-dimensional physical framework integrating numerical simulations with field observations to resolve how different seismic-wave components control deformation anisotropy in water-saturated sediments. We show that horizontally polarized shear waves dominate anisotropic deformation, producing systematically stronger shear and folding on planes oriented perpendicular to wave propagation. This behaviour is quantified using a dimensionless deformation index and fold counts measured on orthogonal profiles. Applying this framework to a well-preserved three-dimensional seismite in the Pamir region, we demonstrate that contrasts in deformation intensity robustly record seismic source direction and enable identification of causative seismogenic faults, together with reconstruction of a sequence of paleo-earthquakes when integrated with chronological constraints. These results establish that near-surface geological deformation can preserve directional information on seismic-wave propagation, opening new opportunities to reconstruct seismic source direction from sedimentary cores and outcrop-scale geological records worldwide.

How to cite: Yang, X., Shi, X., Yang, H., Klinger, Y., Chen, H., Ge, J., Li, F., Liu, X., Yan, Y., and Bai, Z.: Three-dimensional anisotropy of seismite deformation constrains seismogenic fault location, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10546, https://doi.org/10.5194/egusphere-egu26-10546, 2026.

EGU26-10634 | ECS | Orals | TS3.2

Dating Hanging-Wall Colluvial Breccia to Reconstruct the Long-term Normal Fault Evolution in Carbonate Terrains 

Gali Shraiber, Shalev Siman-Tov, Ari Matmon, Tzahi Golan, Naomi Porat, Yael Jacobi, and Perach Nuriel

Normal fault systems within extensional domains often create steep mountain fronts and associated colluvial breccia deposits. These deposits hold an archive of long-term fault activity and landscape evolution, yet they are rarely used to quantify fault slip histories due to their complex nature and dating challenges. In this study, we investigate the Zurim Escarpment in northern Israel, focusing on the Sajur Fault, to reconstruct the long-term morphotectonic history from syn-tectonic colluvial breccia units on the hanging-wall. We integrate U-Pb dating of calcite precipitates and luminescence dating of quartz grains within the breccia matrix to constrain the timing of two breccia depositional phases. Dating results constrain the age of the older breccia phase to ~2.5 Ma, and the younger phase to at least 1.2 Ma. The presence of colluvial breccia at ~2.5 Ma indicates that relief had already developed, constraining the minimum age of escarpment formation. Through clast provenance analysis, we link breccia deposition to the progressive exhumation of the fault footwall. This yielded a long-term slip rate of 0.14±0.02 to 0.15±0.02 mm/yr over the past 2.5 million years, lower than short-term rates derived from cosmogenic dating of fault scraps (0.2–0.5 mm/yr). This discrepancy reflects the temporal dependence of fault slip rates calculations, with values decreasing and stabilizing over longer timescales as they capture the full ratio of seismically active periods to intervening quiescent periods. Our results underscore the potential of syn-tectonic colluvial breccia as a long-term archive for fault activity and landscape evolution in carbonate terrains.

How to cite: Shraiber, G., Siman-Tov, S., Matmon, A., Golan, T., Porat, N., Jacobi, Y., and Nuriel, P.: Dating Hanging-Wall Colluvial Breccia to Reconstruct the Long-term Normal Fault Evolution in Carbonate Terrains, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10634, https://doi.org/10.5194/egusphere-egu26-10634, 2026.

EGU26-10939 | ECS | Orals | TS3.2

Earthquake rupture in a strike slip experiment  

Louis Demange, Pauline Souloumiac, Bertrand Maillot, Salah-Eddine Hebaz, and Yann Klinger

Seismotectonic analogue models provide a valuable complement to seismological, geodetic and paleoseismological-geomorphological approaches for investigating the earthquake cycle. Physical models mainly made with elastic and frictional materials, allow the simulation of multiple seismic cycles under controlled laboratory conditions. Such physical models can reproduce interseismic, coseismic and postseismic deformation. However, all those models include a pre-existing fault, and thus do not necessarily model realistic fault geometries. As a consequence, the influence of geometric complexity—such as fault segmentation, bends, and step-overs—on rupture dynamics and seismic cycle behaviour remains poorly explored in those seismotectonic models.

Here, we present a new analogue seismotectonic model of a strike-slip fault system that allows complex fault geometries to emerge and evolve while producing multiple seismic cycle. The experimental setup consists of two juxtaposed horizontal PVC plates separated by a straight velocity discontinuity, with one plate fixed and the other moving at constant velocity, simulating a vertical basement fault. The overlying medium is composed of three granular layers:  a basal layer of rubber pellets that stores elastic strain, an intermediate rice layer that exhibits stick–slip behavior and represents the seismogenic crust, and an upper frictionally stable sand layer mimicking a non-seismogenic shallow crust.

Surface deformation is monitored with photographs acquired every 2 seconds, corresponding to 25 μm of displacement for the basal plate , and processed using image correlation and dense optical flow methods. Seismic events are detected when surface displacement exceed the imposed basal plate displacement. In addition, recordings made with a high-speed camera at 100 frames per second capture transient surface deformation during rupture propagation. A total of 23 high-speed sequences, each lasting 10 seconds, document coseismic surface deformation associated with earthquake propagation.

We explore the potential of this experimental setup to investigate how rupture characteristics—such as rupture velocity, nucleation and arrest processes— may depend on the evolution of fault geometry and associated off-fault deformation. By quantifying the spatiotemporal distribution of surface deformation and seismic events along evolving fault networks, this approach allows us to investigate how fault segments are activated, temporarily locked, or interact throughout successive stages of the seismic cycle. Moreover, we examine how interseismic deformation reflects the evolving mechanical state and geometry of the fault system, and how this state influences subsequent earthquakes.

How to cite: Demange, L., Souloumiac, P., Maillot, B., Hebaz, S.-E., and Klinger, Y.: Earthquake rupture in a strike slip experiment , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10939, https://doi.org/10.5194/egusphere-egu26-10939, 2026.

EGU26-10956 | ECS | Orals | TS3.2

Insights into fault evolution and rupture dynamics in a strike-slip context from 3D Discrete Element models 

Adélaïde Allemand, Yann Klinger, and Luc Scholtès

Strike-slip continental faults often show complex geometries, inherited from their past history. More particularly, they display branches, bends, and steps, also referred to as geometric asperities. Thus, far from being straight-lined, continental strike-slip faults are characterised by disconnected and misaligned sections, whose length and separating distance vary as the faults mature in time.

The presence of those discontinuities (or complexities) along the fault could affect earthquake rupture dynamics; indeed, the extensional or compressional nature of these discontinuities results in stress heterogeneities along the fault system. In addition, depending on the degree of development of the latter, the deformation at fault complexities can show various levels of localisation, balancing between fault segments well connected by fractures and fault portions dominated by damaged zones where the deformation is distributed. As a consequence, fault complexities often act as nucleation- or end-points for seismic ruptures.

In order to study the effect of fault geometry on earthquake ruptures, we developed a 3D numerical model of an evolving continental strike-slip fault, based on the Discrete Element Method (DEM).

In this model, an initially intact medium is subjected to a strike-slip tectonic regime and, thanks to the DEM capability to explicitly describe progressive failure mechanisms, it evolves through different stages of deformation that eventually lead to the emergence of a structure presenting complexities similar to that of natural faults. We are thus able to analyse the relationship between fault maturity and fault geometry. In addition, multiple local ruptures occur along the fault. Therefore, we can characterise the evolution of the earthquake cycles with geological history: on one hand, for each earthquake, we explore how the rupture is spatially affected by fault complexities; on the other hand, we look at the way successive earthquakes progressively modify the geometry of the fault system. Finally, we compare those observations with natural cases.

How to cite: Allemand, A., Klinger, Y., and Scholtès, L.: Insights into fault evolution and rupture dynamics in a strike-slip context from 3D Discrete Element models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10956, https://doi.org/10.5194/egusphere-egu26-10956, 2026.

Seismic hazard models increasingly rely on detailed active fault databases to explicitly represent earthquake sources and their complex geometries. However, transforming fault-based information into consistent and physically plausible inputs for probabilistic seismic hazard analysis (PSHA) remains a non-trivial and often fragmented task. We present NEXTQUAKE, a modular MATLAB tool designed to bridge this gap by converting an active fault database into a complete, internally consistent seismic hazard input. The first core component of NEXTQUAKE generates a comprehensive catalog of earthquake ruptures starting from the geometry of an active fault system. The algorithm constructs single-fault and multi-fault ruptures while enforcing physical plausibility through a fault-to-fault and subsection-to-subsection connectivity framework. Multi-fault ruptures are generated only among geometrically and kinematically connected faults, dramatically reducing the combinatorial space and ensuring realistic rupture scenarios. Each rupture is described in terms of geometry, area, and magnitude, and is encoded through a sparse subsection–rupture incidence matrix that enables efficient downstream processing. The second component performs an inversion to estimate the expected occurrence rates of all generated ruptures. The inversion integrates geological and geophysical constraints, such as long-term slip rates, and provides a self-consistent set of rupture rates compatible with the fault database. This step allows the direct use of fault-based information within probabilistic frameworks without relying on simplified or ad hoc assumptions. Finally, the third component of NEXTQUAKE translates the rupture catalog and associated rates into fully compliant input files for OpenQuake, enabling seamless integration with state-of-the-art PSHA engines. By automating the entire workflow, NEXTQUAKE offers a transparent, reproducible, and extensible framework for fault-based seismic hazard modeling. NEXTQUAKE is particularly suited for regional-scale applications and for exploring the impact of rupture connectivity assumptions on seismic hazard results.

How to cite: Valentini, A.: NEXTQUAKE: a MATLAB tool to transform an active fault database into seismic hazard input, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11056, https://doi.org/10.5194/egusphere-egu26-11056, 2026.

EGU26-11337 | Orals | TS3.2

Viscoelastic Stress Loading Following the 1999 Earthquakes and Late-Stage Seismicity in the Marmara Sea 

Süleyman S. Nalbant, Fatih Uzunca, Murat Utkucu, and Hatice Durmuş

The 17 August 1999 İzmit (M7.4) and 12 November 1999 Düzce (M7.2) earthquakes ruptured the North Anatolian Fault Zone (NAFZ) in northwestern Türkiye and caused catastrophic damage. The offshore extensions of the central and northern strands of the NAFZ beneath the Sea of Marmara remain seismically active, having produced several Mw≥ 5.0 earthquakes since 2005. In this study, we analyse the spatiotemporal evolution of Coulomb stress changes following the 1999 earthquake doublet and examine their relationship to subsequent moderate earthquakes, including the 2006 Gemlik (Mw5.0), 2019 Silivri (Mw5.7), 2023 Mudanya (Mw5.0), and 2025 Silivri (Mw6.2) events.

Our models indicate that for the 2006 Gemlik and 2023 Mudanya earthquakes, coseismically imposed stress shadows generated by the 1999 ruptures were progressively erased and reversed to positive values by viscoelastic postseismic relaxation in the lower crust and upper mantle. In contrast, at the locations of the 2019 and 2025 Silivri earthquakes, positive coseismic stress changes were substantially amplified by subsequent viscoelastic processes. These results demonstrate that stress perturbations associated with the 1999 mainshocks continue to modulate seismicity along offshore Marmara fault segments over decadal timescales.

In the broader context of the seismic cycle of the Main Marmara Segment, which last ruptured in 1766, the increasing occurrence of moderate-magnitude earthquakes may reflect a transition toward a late-stage, critically stressed regime. Our results suggest that long-lived viscoelastic stress transfer following the 1999 earthquakes has imposed an additional stress load on an already mature seismic cycle, potentially accelerating its progression toward failure. Accounting for such persistent, time-dependent stress interactions is therefore essential for refining time-dependent earthquake hazard assessments in this densely populated region.

How to cite: Nalbant, S. S., Uzunca, F., Utkucu, M., and Durmuş, H.: Viscoelastic Stress Loading Following the 1999 Earthquakes and Late-Stage Seismicity in the Marmara Sea, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11337, https://doi.org/10.5194/egusphere-egu26-11337, 2026.

EGU26-11580 | ECS | Posters on site | TS3.2

Numerical Modelling of Fault-Slip-Induced Satellite Gravity Signals in a 3D Viscoelastic Earth: Application to the Japanese Subduction System 

Rajesh Parla, Isabelle Panet, Hom Nath Gharti, Roland Martin, Dominique Remy, and Bastien Plazolles

The spatio-temporal variations of the Earth’s gravity field recorded by satellites have been shown to provide unique insight into mass redistributions during and after major subduction-zone earthquakes, and to reveal anomalous signals preceeding two great ruptures, attributed to rapid aseismic deformations of subducted plates. Understanding these gravity signatures is important for studying subduction system dynamics throughout the earthquake cycle and for improving regional seismic risk assessment. Physics-based numerical simulations are therefore needed in order to model pre- to post-seismic satellite gravity signals, taking into account the 3D structure of the subducting zone, including lateral heterogeneities in the mantle rheology and lateral variations in crustal thickness. In this study, we apply a novel numerical approach to simulate gravity perturbations induced by fault dislocations in a 3D viscoelastic Earth using a Spectral-Infinite-Element (SIE) method, implemented in the SPECFEM-X numerical code. Considering examples of dislocation within a subducted slab, we examine the sensitivity of the surface gravity signals to 3D slab geometry and material structure, including the effects of low-viscosity layers, mantle wedge and cold nose. This approach enables us to investigate the sources of the pre-seismic gravity anomalies prior to the 2011 Mw 9.1 Tohoku earthquake through realistic 3D Earth models and state-of-the-art simulation setups. The findings of this study underscore the importance of numerical simulations in gravitational geodesy as well as in seismic hazard assessment.

How to cite: Parla, R., Panet, I., Gharti, H. N., Martin, R., Remy, D., and Plazolles, B.: Numerical Modelling of Fault-Slip-Induced Satellite Gravity Signals in a 3D Viscoelastic Earth: Application to the Japanese Subduction System, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11580, https://doi.org/10.5194/egusphere-egu26-11580, 2026.

EGU26-11605 | ECS | Posters on site | TS3.2

Coseismic Surface Deformation Characteristics of the 1915 M7.0 Sangri Earthquake in Tibet 

Junxiang Qiao, Haoyue Sun, and Xin Wang

The spatial distribution and deformation characteristics of coseismic surface rupture zones are fundamental to understanding the rupture behavior of strong earthquakes. They provide critical insights for predicting the extent, scale, and degree of deformation of future events, which is of great significance for assessing the magnitude of potential seismic hazards.

The December 3, 1915, M7.0 Sangri earthquake in the Woka Graben (northern Cona-Woka Rift) is the region’s most recent major seismic event. Historical records place the epicenter near Zangga, identifying the Eastern Boundary Fault (EBF) as the primary seismogenic structure. However, its remote, high-altitude location and coarse legacy satellite imagery have left details undocumented and source parameters poorly constrained. To address this, we integrated UAV-derived centimeter-scale Digital Surface Models (DSM), orthomosaics, and field investigations. This enabled multi-scale, multi-perspective analysis of fault traces, surface rupture geometry, and coseismic deformation.

Refined mapping reveals that the seismogenic EBF manifests as a continuous, single-branch structure with a total length of approximately 60 km. The fault trace is well-defined and can be divided into northern and southern segments by the Delimuqu River. The northern segment extends ~29km in a nearly N-S direction with a westward dip, while the southern segment extends ~31 km with a NNE strike and a NW dip. A distinct coseismic surface rupture zone, ~35 km in length, developed primarily along the entire northern segment and the northern part of the southern segment of the EBF. Field measurements revealed a maximum coseismic vertical displacement of ~2.1m.

Furthermore, we utilized a MATLAB-based displacement measurement program to perform quantitative extraction of cumulative offsets and Cumulative Offset Probability Density (COPD) analysis across 225 investigation sites, yielding an average coseismic vertical displacement of ~0.79 m. Additionally, a fault scarp diffusion age modeling program was employed to constrain the extent of the coseismic surface rupture based on morphological degradation. Analysis of 362 measurement sites via COPD indicated an average diffusion age of 2.05 ± 0.88 kt for the coseismic scarps. The integration of spatial distributions for minimum mean diffusion ages and cumulative vertical displacements allowed us to quantitatively define the coseismic surface rupture length to ~32 km. This result is in excellent agreement with the ~35 km length derived from remote sensing interpretation, validating the reliability of the estimated rupture scale. Using empirical scaling relationships based on the obtained rupture length and the average/maximum vertical displacements, we re-estimated the earthquake magnitude to be Mw 6.71~6.84, highlighting the high seismic potential of the EBF. This study fills a critical gap in the detailed investigation of the coseismic surface rupture of the 1915 Sangri earthquake and underscores the significant utility of high-resolution topographic data in active tectonics research.

How to cite: Qiao, J., Sun, H., and Wang, X.: Coseismic Surface Deformation Characteristics of the 1915 M7.0 Sangri Earthquake in Tibet, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11605, https://doi.org/10.5194/egusphere-egu26-11605, 2026.

EGU26-12056 | ECS | Posters on site | TS3.2

3-D Discrete Element Modeling of Continental Fault System Evolution Under Oblique Boundary Conditions 

Adarsh Dwivedi, Yann Klinger, and Luc Scholtès

Oblique displacement in continental tectonic setting often leads to complex fault systems that incorporate both dip-slip and strike-slip motion, with fault geometry and seismic activity developing across subsequent earthquake cycles. Understanding how boundary conditions influence fault growth, rupture dynamics, and off-fault deformation is an ongoing challenge in tectonics and earthquake physics. In this study, we are using three-dimensional discrete element models to analyze the evolution of continental fault systems under oblique boundary conditions.Specifically, we employ a numerical sandbox that represents the continental crust as a brittle layer where deformation can localize as a result of fracture nucleation, propagation and coalescence, without any a priori assumptions on its spatio-temporal evolution. Transtensional and transpressional loadings are applied through combined normal and shear components of deformation. Our simulations show cyclic stick-slip behavior, defined by periods of elastic responses followed by fault ruptures. Thanks to the model’s capability, we analyze the evolution of the emerging fault geometry, the ruptures extent, as well as slip partitioning throughout the simulated earthquake cycles. Particular emphasis is placed on the spatial distribution of damage, the development of fault-related topography on the surface, and the role of obliquity in controlling rupture propagation. Our findings show strong relationships between imposed boundary conditions, fault system configuration, and seismic rupture characteristics.

How to cite: Dwivedi, A., Klinger, Y., and Scholtès, L.: 3-D Discrete Element Modeling of Continental Fault System Evolution Under Oblique Boundary Conditions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12056, https://doi.org/10.5194/egusphere-egu26-12056, 2026.

EGU26-13346 | ECS | Orals | TS3.2

Afterslip following the 2023 Mw7.8 and Mw7.6 Kahramanmaraş earthquakes: observations and modeling 

Cyril Lacroix, Baptiste Rousset, Frédéric Masson, Paul Dérand, Romain Jolivet, Ali Özkan, and Hakan Hasan Yavaşoğlu

On February 6, 2023, two earthquakes of magnitude Mw7.8 and Mw7.6 struck in South Türkiye. The first mainshock occurred along the East Anatolian fault, at the boundary between the Anatolian and Arabian plates, and was followed 9 hours later by a second one on a secondary fault system to the North. The importance of such continental earthquakes and the relatively good data coverage of the region present an unique opportunity to investigate post-seismic deformation.

To study afterslip, corresponding to post-seismic transient aseismic slip, we use a combination of ground deformation measurements, including Sentinel-1 InSAR timeseries (6 tracks covering almost 2 years after the earthquakes) and GNSS (more than 40 permanent stations and 60 campaign sites). The cities of Hassa and Gölbaşı, located on the East Anatolian fault, are investigated in detail using 8 continuous GNSS stations installed across the fault 6 months after the earthquakes.

While the large surface imprint of the surface deformation, with significant displacements more than 200 km away from the fault, and our inability to model it with fault slip points toward the dominance of a visco-elastic processus, clear markers of shallow afterslip are visible. In the Pütürge segment, located at the tip of the first earthquake’s coseismic rupture, InSAR data reveals a cumulative surface offset 20 months after the earthquake of about 10 cm due to shallow afterslip. Other segments affected with afterslip have been identified in the eastern part of the rupture of the second earthquake, accounting for several centimeters of slip over 20 months. Our local GNSS networks in Hassa and Gölbaşı reveal the smaller scale complexity of post-seismic surface deformation near the fault. In Gölbaşı, subsidence of more than 2 cm/year is highlighted in the pull-apart basin, while horizontal GNSS displacements suggest possible shallow aseismic slip happening at the southern end of the basin.

We model afterslip on the fault by jointly inverting InSAR and GNSS data, minimizing the least squares criterion. Afterslip is concentrated around the coseismic rupture zone, accompanied by important aftershock activity. The Pütürge segment appears as a seismic barrier, having stopped both Mw6.8 2020 Elazığ earthquake to the East and Mw7.8 2023 Kahramanmaraş earthquake to the West, possibly because of the fault geometry and/or heterogeneous coupling. Future efforts will be directed towards the evolution of afterslip with time and its interplay with aftershocks, including visco-elastic relaxation models. These results help us better understand the relationship between the different phases of the seismic cycle.

How to cite: Lacroix, C., Rousset, B., Masson, F., Dérand, P., Jolivet, R., Özkan, A., and Yavaşoğlu, H. H.: Afterslip following the 2023 Mw7.8 and Mw7.6 Kahramanmaraş earthquakes: observations and modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13346, https://doi.org/10.5194/egusphere-egu26-13346, 2026.

EGU26-14323 | Orals | TS3.2

Burstiness and memory of large subduction earthquakes: insights from paleoseismology and analogue modelling 

Fabio Corbi, Elvira Latypova, Giacomo Mastella, Francesca Funiciello, Silvia Brizzi, and Simona Guastamacchia

Constraining the timing of large subduction earthquakes remains a fundamental yet unresolved problem in seismic hazard assessment. Although paleoseismic records from many subduction margins suggest predominantly quasi-periodic recurrence of great earthquakes, the large variability observed among different segments and regions raises the question of whether such patterns reflect intrinsic megathrust behavior or, instead, the limitations of the available records. Here we investigate the robustness and interpretability of earthquake recurrence metrics by combining global paleoseismic datasets with scaled seismotectonic models of the subduction megathrust seismic cycle.

We characterize earthquake recurrence using two complementary statistics: burstiness (B), which quantifies the degree of periodicity and clustering of inter-event times, and the memory coefficient (M), which captures temporal correlations between consecutive recurrence intervals. Mapping paleoseismic records from multiple subduction zones onto the M–B plane reveals that most segments exhibit quasi-periodic behavior (B < 0), but span a wide range of memory values, from strongly negative to strongly positive. Notably, this diversity shows no systematic dependence on subduction rate, earthquake rate, or record length, and adjacent segments along the same margin may occupy markedly different regions of the M–B plane.

To assess whether this apparent variability reflects differences in fault dynamics or observational bias, we analyze long, continuous earthquake sequences generated by scaled seismotectonic models. Despite large contrasts in asperity number, size, and along-strike strength heterogeneity, experimental sequences cluster within a relatively narrow domain of the M–B plane. Through controlled subsampling tests, we show that catalog incompleteness, limited along-strike coverage, and short observation windows can substantially shift M and, to a lesser extent, B. 

The analysis of experimental data provides useful constraints on the limits of our ability to infer long-term earthquake recurrence from paleoseismic records, with important implications for probabilistic seismic hazard assessment.

How to cite: Corbi, F., Latypova, E., Mastella, G., Funiciello, F., Brizzi, S., and Guastamacchia, S.: Burstiness and memory of large subduction earthquakes: insights from paleoseismology and analogue modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14323, https://doi.org/10.5194/egusphere-egu26-14323, 2026.

EGU26-15813 | Orals | TS3.2

DEM Modelling-Based Insights into the Controlling Factors of Strike-Slip Fault Segmentation 

Liqing Jiao, Yang Jiao, and Yueqiao Zhang

Strike-slip shearing is widespread in the brittle crust and is typically expressed as segmented rupture zones with characteristic spacing. Yet, the key factors controlling this geometric pattern remain poorly understood. In this study, we use discrete element method (DEM) simulations to systematically explore the fundamental physical and tectonic controls on fault segment spacing in strike-slip systems. Our results show that spacing is influenced by both physical and tectonic factors. Physically, spacing increases with crustal thickness and strength, but decreases with density and gravitational acceleration. A near-linear relationship emerges between the ratio of spacing length to thickness and the ratio of strength to the combined effects of density, gravity, and thickness. Tectonically, spacing is reduced by increasing thrust components but enlarged by extensional components. Pre-existing weak zones strongly localize rupture, while surface topography modulates rupture propagation, with segments preferentially forming in lower-elevation areas. These results offer new insights into the mechanics of segmented strike-slip ruptures on Earth and other planetary bodies and provide a framework for better assessing natural hazard risks.

How to cite: Jiao, L., Jiao, Y., and Zhang, Y.: DEM Modelling-Based Insights into the Controlling Factors of Strike-Slip Fault Segmentation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15813, https://doi.org/10.5194/egusphere-egu26-15813, 2026.

EGU26-15880 | ECS | Posters on site | TS3.2

High-resolution Coral Geodesy in the Solomon Islands 

Mehmet Ege Karaesmen, Luc Lavier, and Frederick Taylor

The classical earthquake cycle is commonly described as alternating between long periods (decades to centuries) of interseismic locking and brief episodes (seconds) of coseismic rupture. However, increasingly dense geodetic observations from recent megathrust earthquakes reveal a more complex spectrum of transient deformation processes that challenge this binary framework. The New Georgia Group in the Solomon Islands provides a unique natural laboratory to investigate these processes, where the Woodlark Basin subducts beneath the Solomon Arc and has generated large megathrust earthquakes, including the 1936 Mw 7.9 and 2007 Mw 8.1 events.

The close proximity of the islands to the trench allows Porites corals to serve as high-resolution recorders of vertical ground motion. While coral morphology has long been used to identify coseismic uplift, we introduce a novel approach that combines coral morphology with stable isotope analysis (δ¹³C and δ¹⁸O) to quantify relative sea-level (RSL) variations at annual resolution. We first assess the robustness of the relationship between coral water depth and δ¹³C using 141 new samples collected across a range of depths formed within the same time interval. For depths between 170 and 110 cm below sea level, δ¹³C exhibits a strong linear correlation with water depth (R² = 0.982), while shallower samples display a non-linear response.

We then apply this RSL proxy to a 692-sample coral time series spanning 1928–2012 and validate the reconstructed RSL against available tide-gauge records. The 2007 Mw 8.1 earthquake is clearly resolved, with coral morphology recording ~70 cm of coseismic uplift expressed as a pronounced die-down surface, accompanied by a δ¹³C excursion exceeding 2‰. The 1936 Mw 7.9 event is similarly captured by a distinct δ¹⁸O anomaly, with postseismic relaxation observed consistently along two independent drilling transects.

Beyond discrete coseismic signals, the record reveals multi-year to decadal periods of uplift and subsidence that we interpret as complex interseismic deformation. In particular, we identify intervals consistent with slow slip activity during 1955–1964, 1977–1986, and 1999–2002. These results demonstrate that stable isotope measurements in corals provide a powerful bridge between instrumental geodesy and paleoseismology, enabling a continuous, high-resolution view of subduction-zone deformation and stress evolution across the full earthquake cycle.

How to cite: Karaesmen, M. E., Lavier, L., and Taylor, F.: High-resolution Coral Geodesy in the Solomon Islands, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15880, https://doi.org/10.5194/egusphere-egu26-15880, 2026.

EGU26-17057 | Posters on site | TS3.2

Linking Fault Geometric Complexity and Cumulative Displacement with Seismic Behavior: Insights from the Gran Sasso Fault System (Central Apennines, Italy) 

houda delleci, Lucilla Benedetti, Magali Riesner, Giulio Di Toro, Michele Fondriest, and John Gallego Montoya

Active normal faults in the Central Apennines accommodate ongoing crustal extension and have generated significant earthquakes (up to Mw ~7) during historical and instrumental times. However, several fault systems, including the Gran Sasso fault system (GSFS), lack documented surface-rupturing earthquakes, raising questions about their structural maturity, role in accommodating the extension in this region, and their potential to generate future large-magnitude events.

Here, we investigate the relationship between fault geometry, cumulative displacement, and slip rate along the Gran Sasso fault system located 19km north of L’Aquila, a system consisting of two major normal faults with an overall length of ~46 km. These include(i) the Campo Imperatore fault, consisting of two segments measuring roughly 20 km and 8 km, and (ii) the Assergi fault, which extends about 18 km along the western flank of the Gran Sasso massif. Both faults exhibit a consistent average W-E orientation with secondary structure tending WNW-ESE. Our aim is to assess the structural maturity and seismic significance of the GSFS within the broader Apennine fault network.

Using high-resolution Pleiades satellite imagery combined with existing geological maps and field observation, we mapped in detail the active fault trace and identified displaced geomorphic markers. The analysis focuses on two main fault segments, the Campo Imperatore and Assergi segments, along which a well-preserved Holocene fault scarp is continuously expressed. Scarp height was measured accurately along strike using several complementary approaches, including field-based observations, topographic profiles extracted from high-resolution DEMs, and the automated ScarpLearn algorithm (Pousse et al., 2022), which identifies and quantifies fault scarp morphology together with associated uncertainties. Preliminary results indicate that vertical displacement varies between ~2 and 16 m, locally reaching up to ~20 m along the Campo Imperatore segment. These results are analyzed in relation to fault architecture to assess how geometric complexities, such as relay zones and step-overs, influence displacement distribution along strike

Field investigations and detailed mapping along the Campo Imperatore fault allowed the identification of three key sites where fluvial terraces and glacial moraines are displaced and can be used as geomorphic markers of fault slip. Samples were collected for ^36Cl cosmogenic exposure dating of these surfaces. When combined with measured offsets, these exposure ages provide constraints on average late Quaternary slip rates and on the long-term activity of the fault, under the assumption that the dated surfaces record cumulative displacement since their abandonment.

How to cite: delleci, H., Benedetti, L., Riesner, M., Di Toro, G., Fondriest, M., and Montoya, J. G.: Linking Fault Geometric Complexity and Cumulative Displacement with Seismic Behavior: Insights from the Gran Sasso Fault System (Central Apennines, Italy), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17057, https://doi.org/10.5194/egusphere-egu26-17057, 2026.

EGU26-17450 | Posters on site | TS3.2

Paleoseismology of the Roccapreturo Fault (Central Apennines): Insights from Antithetic Fault Trenching and Image-Enhanced Analysis 

Magali Riesner, John Gallego-Montoya, Lucilla Benedetti, Stefano Pucci, Francesca Romana Cinti, Paolo Boncio, Daniela Pantosti, Alessio Testa, Matthieu Ferry, Stephane Baize, and Bruno Pace

The Roccapreturo Fault (RF) is a 9 km-long NW-SE normal fault forming one of the major segments of the Middle Aterno Valley Fault system, located 20 km south of L’Aquila in the Central Apennines (Italy). Despite its clear seismogenic potential, no earthquakes have been documented in historical sources. Large earthquakes on such structures typically have time intervals of several millennia, making paleoseismology crucial for constraining their long-term seismic behavior. The RF exhibits 150–250 m-high triangular facets and a 10 m-high semi-vertical fault scarp that cuts the Cretaceous limestone sedimentary sequence and delineates the main fault trace. North of Roccapreturo village, Quaternary colluvial deposits and alluvial fans feed a small intermontane basin, bounded by a 25-m-high ridge most probably related to the cumulative displacement along an antithetic fault subparallel to the main fault. We excavated two paleoseismological trenches across this antithetic fault, where a refined sedimentary record enhances the preservation of coseismic deformation. An additional trench was excavated ~1 km south, at the base of the main fault scarp.

Trenches were logged using standard stratigraphic, structural, and event-identification criteria. Event ages were constrained through radiocarbon dating of 23 bulk-sediment and charcoal samples. To complement conventional trench analysis, we implemented an integrated workflow combining conventional paleoseismology with pixel-based image enhancement. This approach exploits multi-temporal orthophotography datasets acquired at different spatial resolutions and times. Photogrammetric products (orthomosaics, true- and false-color RGB composites, 3D textured point clouds, and raster derivatives) were integrated into a georeferenced multi-layer stack to support post-field interpretation and independent validation of trench observations.

In the trenches across the antithetic fault, the basal stratigraphy consists of fine-grained marsh deposits faulted and folded against fractured and brecciated limestone bedrock. These units are overlain by clast-supported colluvial sequences containing wedges that record cumulative vertical displacements of up to ~70 cm, defining multiple paleoearthquake horizons. Three to four surface-rupturing events were identified in the antithetic fault trenches, with clustered ages of 0–1.7 ka, 4–8 ka, 8–13 ka, and 15–21 ka. In contrast, the trench excavated at the base of the main scarp preserves only a single recent event within colluvial deposits, consistent with the youngest event recorded in the antithetic fault trenches.

Previous studies along the main RF focused on cosmogenic dating of the bedrock scarp, estimating Middle Pleistocene slip rates of 0.2–0.3 mm/yr, and on trenching at alluvial-fan intersections. Two Holocene surface-rupturing events (2–8 ka) were identified, indicating a recurrence of about 2 ka and magnitudes up to Mw 6.5. The earthquake events that yielded in our trenches correlate well with previous results, extending the seismic record of the RF into the Late Pleistocene. Together, these results are crucial for constraining the timing and recurrence of surface-rupturing events and for assessing the role of antithetic faults in accommodating distributed deformation within the fault system. In addition, integrating image-enhancement techniques improves the visualization of subtle deformation and stratigraphic relationships, reduces interpretative uncertainty, and provides a scalable, reproducible framework that effectively complements classical paleoseismological trenching.

How to cite: Riesner, M., Gallego-Montoya, J., Benedetti, L., Pucci, S., Cinti, F. R., Boncio, P., Pantosti, D., Testa, A., Ferry, M., Baize, S., and Pace, B.: Paleoseismology of the Roccapreturo Fault (Central Apennines): Insights from Antithetic Fault Trenching and Image-Enhanced Analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17450, https://doi.org/10.5194/egusphere-egu26-17450, 2026.

EGU26-18093 | Orals | TS3.2

When subduction changes its grip: cycle-to-cycle variability in interseismic coupling and coseismic slip 

Elvira Latypova, Jonathan Bedford, Fabio Corbi, Giacomo Mastella, Francesca Funiciello, Simona Guastamacchia, and Silvio Pardo

Identifying frictionally locked regions of subduction megathrusts from geodetic observations remains a challenging task in tectonic geodesy. Natural geodetic records typically capture only a fraction of seismic cycles, restricting our ability to assess temporal variations in interseismic coupling and their relationship to frictionally locked regions on subduction interfaces, commonly referred to as asperities. Clarifying this relationship is important, because interseismic coupling is widely used as an indicator of seismic potential, but coupled regions may include both mechanically locked asperities and surrounding unlocked regions. 

Scaled seismotectonic models provide an effective framework to investigate these processes, by simulating hundreds of seismic cycles within a short time interval under controlled laboratory conditions, with predefined asperity distributions and high-resolution deformation monitoring. 

Here, we explore the spatiotemporal variability of interseismic coupling, coseismic slip and their connection to predefined asperities using Foamquake, a well-established 3D seismotectonic model, which simulates megathrust seismic cycles.

Through kinematic inversions of surface deformation, we derive cycle-by-cycle maps of interseismic coupling and coseismic slip and analyse their statistical behavior across models with different asperity configurations and applied normal stress. Our results show pronounced cycle-to-cycle variability in interseismic coupling, even within asperity regions, with highly coupled areas systematically extending beyond the asperity boundaries. Coseismic slip shows a positive but highly scattered correlation with preceding interseismic coupling, suggesting that while coupling is a necessary condition for large slip, it alone does not determine rupture magnitude.

How to cite: Latypova, E., Bedford, J., Corbi, F., Mastella, G., Funiciello, F., Guastamacchia, S., and Pardo, S.: When subduction changes its grip: cycle-to-cycle variability in interseismic coupling and coseismic slip, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18093, https://doi.org/10.5194/egusphere-egu26-18093, 2026.

EGU26-18225 | Posters on site | TS3.2

How to define the earthquake loading medium: an interdisciplinary approach 

Carolina Giorgetti and Cristiano Collettini

Since Reid formulated the elastic rebound theory in the early 20th century to describe earthquakes in brittle faulting, fault systems have been widely represented by spring–slider models, both in theoretical frameworks and laboratory experiments. From a different perspective, structural geology has long documented fault systems as geometrically complex structures, reflecting the heterogeneous physical properties of different lithologies. These systems are characterised by multiple slip surfaces and secondary fault splays and comprise large volumes of highly damaged rocks. Such damaged volumes are effectively part of the loading medium that is commonly conceptualised, in simplified models, as an elastic spring.

Over the past decades, a wealth of seismological and geodetic observations has shown that these damaged crustal volumes actively deform inelastically during the seismic cycle, rather than merely storing elastic energy. In parallel, numerical models indicate that off-fault damage can account for a significant portion of the earthquake energy budget. Together, these observations challenge the classical representation of the fault loading medium as purely elastic.

Here, we integrate observations spanning outcropping fault-zone descriptions, seismicity catalogues, and laboratory observations to explore how the earthquake loading medium could be more realistically defined and described in natural fault systems. We focus on well-studied seismogenic normal faults in Italy, namely the Gubbio and Norcia faults, where a long-standing and extensive knowledge of the involved lithologies is combined with a high-resolution fault image obtained by both high-quality outcrop exposure and enhanced seismological catalogues, and where the involved rocks have been extensively studied in the laboratory. By adopting this interdisciplinary perspective, we aim to better constrain the nature of the loading medium toward a better estimation of the forcing imbalance that is fundamental to earthquake nucleation.

How to cite: Giorgetti, C. and Collettini, C.: How to define the earthquake loading medium: an interdisciplinary approach, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18225, https://doi.org/10.5194/egusphere-egu26-18225, 2026.

EGU26-18883 | ECS | Orals | TS3.2

FASTDASH: an implementation of 3-D earthquake cycle simulation on complex fault systems using the boundary element method accelerated by H-matrices 

Michelle Almakari, Jinhui Cheng, Harsha Bhat, Brice Lecampion, and Carlo Peruzzo

Major fault systems are inherently complex, including geometric features such as multiple interacting fault segments and variations in strike, dip, and depth. Fault geometries can be effectively reconstructed through field observations and seismic monitoring. Many studies have demonstrated that this geometric complexity plays an important role in controlling the initiation, arrest, and recurrence of both seismic and aseismic slip. In particular, 3D variations in fault geometry cannot be neglected.

However, the vast majority of slip-dynamics models are conducted on planar faults due to algorithmic limitations. To overcome this restriction, we develop a 3D quasi-dynamic slip-dynamics model capable of simulating arbitrarily complex fault geometries. In boundary-element methods, the elastic response to fault slip is computed through the multiplication of a dense matrix with a slip rate vector, which are computationally expensive. We accelerate these calculations using hierarchical matrices (H-matrices), reducing the computational complexity from O(N^2) to O(NlogN), where N is the number of elements. The H-matrix parameters provide explicit control over the trade-off between computational efficiency and accuracy.

In our framework, fault geometry is fully arbitrary and discretized using triangular elements. Fault slip is governed by rate-and-state friction laws and loaded by either stressing rates or plate rate. This approach enables efficient simulation of the spatiotemporal evolution of slip and stress on complex fault systems over multiple earthquake cycles.

We validate the model against analytical solutions for static cracks and through a numerical benchmark (SCEC SEAS BP4). Finally, we apply the method to a realistic fault system with complex geometry that was reactivated during the 2023 Kahramanmaraş–Türkiye earthquake doublet. The results highlight the model’s ability to generate complex earthquake sequences driven solely by fault geometry, without including additional complexities such as rheological, frictional, or fluid-interaction effects.

How to cite: Almakari, M., Cheng, J., Bhat, H., Lecampion, B., and Peruzzo, C.: FASTDASH: an implementation of 3-D earthquake cycle simulation on complex fault systems using the boundary element method accelerated by H-matrices, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18883, https://doi.org/10.5194/egusphere-egu26-18883, 2026.

EGU26-19222 | ECS | Posters on site | TS3.2

Quality evaluation of assimilation-based forecast of rate-and-state governed fault analog 

Bharath Shanmugasundaram, Harsha Bhat, and Romain Jolivet

During an earthquake, the frictional resistance of a fault suddenly drops to release the elastic energy that has been accumulating over decades to centuries. In addition to the steady increase of stress on faults due to tectonics, external perturbations have been shown to modulate the fault behavior over a wide range of time scales. The spring block slider model following rate-and-state friction framework with velocity-weakening behavior undergoing periodic perturbations has been known to host complex stick-slip events ranging from fast earthquakes to slow earthquakes, making it a good analog of a simple fault. Accurate characterization of system state and tidal forcing parameters is critical for understanding the triggering mechanisms and ultimately improving seismic hazard assessment. In this work, we employ ensemble-based data assimilation techniques to carry out state and joint state-parameter estimation in a tidal modulated spring slider. We perform twin experiments to estimate the tidal perturbation parameters such as period and amplitude. In this scenario, we compare the iterative ensemble Kalman smoother (I-EnKS) with ensemble Kalman filter (EnKF) variants for joint state-parameter estimation. Using the smoothed estimates, we assess forecast quality by evaluating prediction accuracy over multiple recurrence intervals. To account for model uncertainties, we incorporate additive stochastic forcing to examine its effect on state-parameter estimation and forecast accuracy.

How to cite: Shanmugasundaram, B., Bhat, H., and Jolivet, R.: Quality evaluation of assimilation-based forecast of rate-and-state governed fault analog, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19222, https://doi.org/10.5194/egusphere-egu26-19222, 2026.

EGU26-19316 | Posters on site | TS3.2

Active Tectonics and Paleoseismology of an Extensional Basin: Implications from the Büyük Menderes Graben (Western Anatolia, Türkiye) 

Akın Kürçer, Çağatay Çal, Oğuzhan Yalvaç, Halil Gürsoy, and Hasan Elmacı

Western Anatolia represents one of the most active continental extensional domains within the Alpine–Himalayan orogenic system. Ongoing NNE–SSW extension has produced a system of E–W–trending grabens and half-grabens controlled by active normal faults. These basins provide natural laboratories to investigate the interaction between fault-controlled deformation, sedimentary basin evolution, and seismic hazard. A key characteristic of such extensional basins is the presence of thick, unconsolidated basin fills overlying competent basement rocks. This strong mechanical contrast promotes seismic wave trapping and amplification, leading to prolonged ground-motion duration and increased shaking intensity. Similar basin-related effects have been documented in other extensional and transtensional settings worldwide (e.g., the Basin and Range Province, Central Apennines, and the Aegean region), highlighting their importance for seismic risk in densely populated areas.

The Büyük Menderes Graben is one of the largest and most mature extensional basins in Western Anatolia and hosts several major population centers. Paleoseismological investigations carried out on the main basin-bounding normal faults reveal repeated surface-rupturing earthquakes during the Holocene. These data show that fault segmentation, fault length, and basin geometry play a primary role in controlling earthquake magnitude, rupture characteristics, and recurrence patterns. At a regional scale (~100 km), several active faults have the potential to generate moderate to large earthquakes (Mw ~6.0–7.1). The combined effects of distributed fault deformation and basin amplification imply that seismic hazard in extensional provinces cannot be assessed solely based on proximity to individual faults. Instead, an integrated approach that considers fault interaction, basin geometry, and site effects is required.

In this study, trench-based paleoseismological investigations were carried out along the İncirliova, Umurlu, and Atça segments forming the northern margin of the Büyük Menderes Graben (BMG). In trenches excavated along all three segments, strong evidence was obtained for Holocene earthquakes that produced surface faulting. Preliminary findings suggest that the 22 February 1653 Menderes Valley earthquake (Ms6.7) may have originated from the İncirliova Segment, whereas the 20 September 1899 Menderes Valley earthquake (Ms6.9) was likely generated by the Umurlu and Atça Segments.

This study synthesizes active tectonic observations, paleoseismological trench data, and basin-scale geological constraints from the Büyük Menderes Graben to highlight how extensional basins amplify seismic risk beyond simple fault-based models. The results have broader implications for seismic hazard assessment in other active continental rift and graben systems worldwide, particularly where rapidly growing urban areas are built on young sedimentary basins.

How to cite: Kürçer, A., Çal, Ç., Yalvaç, O., Gürsoy, H., and Elmacı, H.: Active Tectonics and Paleoseismology of an Extensional Basin: Implications from the Büyük Menderes Graben (Western Anatolia, Türkiye), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19316, https://doi.org/10.5194/egusphere-egu26-19316, 2026.

EGU26-19344 | ECS | Orals | TS3.2

Using dense 36Cl profiles to assess the seismic history of the Roccapreturo Fault (Italy)  

Maureen Llinares, Lucilla Benedetti, Ghislain Gassier, and Magali Riesner

The Roccapreturo fault, part of the Middle Aterno Valley Fault system in the central Apennines (Italy), is a key structure for understanding the region’s seismic hazard. Despite evidence of Quaternary activity, its Holocene seismic history remains poorly constrained, with no historical earthquakes directly attributed to this fault. In this study, high- and low-resolution 36Cl cosmogenic nuclide profiles from five sites along the Roccapreturo limestone fault scarp were used to reconstruct the seismic history of this fault. The seismic history was constrained using PyMDS inversion algorithm (Llinares et al., 2025), which relies on Markov Chain Monte Carlo (MCMC) approach to infer the timing and slip of past surface-rupturing earthquakes.

Our results indicate at least five major seismic events over the last ~18,000 years, with coherent clusters at ~5 ka, ~3.5 ka, ~2–3 ka, ~1 ka, and <0.5 ka BP on at least two sites. The most recent event, dated at ~300 years BP, could correspond to a previously unattributed historical earthquake. Slip Rates (SRs) over the Pleistocene, estimated from high resolution profiles, range from 0.1 to 0.4 mm/yr, which is consistent with previous studies (Falcucci et al., 2015; Tesson et al., 2020) and InSAR data (Daout et al., 2023).  SRs over the Holocene are higher (~1–2 mm/yr), suggesting temporal variability. The study also discusses methodological advances, including the value of dense sampling, the use of statistical changepoint detection, and the integration of fuzzy statistics to address uncertainties in seismic history derived from 36Cl dataset from limestone fault scarp.

These findings provide new constraints on the seismic behavior of the Roccapreturo fault, highlight the importance of multi-site and high-resolution approaches, and underscore the need for further paleoseismological and historical investigations to refine the seismic hazard assessment in the central Apennines.

How to cite: Llinares, M., Benedetti, L., Gassier, G., and Riesner, M.: Using dense 36Cl profiles to assess the seismic history of the Roccapreturo Fault (Italy) , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19344, https://doi.org/10.5194/egusphere-egu26-19344, 2026.

EGU26-19393 | Posters on site | TS3.2

Velocity-Dependent Friction and Its Role in the Evolution of Surface Deformation and Topography in Strike-Slip Fault Systems 

Ernst Willingshofer, Ehsan Kosari, Lise Wassens, and Ylona van Dinther

Strike-slip faults accommodate plate motion through a coupled spectrum of abrupt seismic rupture and distributed, aseismic creep that coexist and interact within the same fault system. Yet the surface expression of these behaviours remains poorly constrained, largely because the short-term physics of frictional instability and the long-term construction of fault-zone morphology are rarely observed within a single framework. Here, we address this gap using seismotectonic analogue experiments designed to isolate how velocity-dependent (velocity-weakening and velocity-strengthening) and neutral frictional regimes govern both transient and cumulative deformation in strike-slip systems. The experiments reproduce hundreds of analogue earthquake cycles along a laboratory strike-slip fault system to build topography while simultaneously measuring shear force, acoustic emissions, and full-field surface displacements. By systematically modifying fault material properties and boundary conditions, we analyse their mechanical and geometric consequences.

We argue that the distinction between velocity-weakening, neutral, and strengthening friction is not merely a control on whether earthquakes occur but also organizes fault-zone architecture. In the velocity-weakening zone, deformation is expected to concentrate episodically into narrow, migrating shear bands that imprint discontinuous, step-like surface relief. In contrast, velocity-strengthening and velocity-neutral regimes should promote diffuse surface strain, topographic gradients, and a cumulative memory of stable slip. Investigating the interaction between these regimes provides a mechanical explanation for natural strike-slip faults that often display coexisting seismic segments and creeping sections. By linking fault frictional heterogeneity to measurable surface deformation patterns, we aim to contribute to presenting a mechanical and morphological framework for strike-slip fault evolution.

How to cite: Willingshofer, E., Kosari, E., Wassens, L., and van Dinther, Y.: Velocity-Dependent Friction and Its Role in the Evolution of Surface Deformation and Topography in Strike-Slip Fault Systems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19393, https://doi.org/10.5194/egusphere-egu26-19393, 2026.

EGU26-19397 | ECS | Orals | TS3.2

Advancing Paleoseismology with Integrated Hyperspectral and Multi-Sensor Approaches: Enhanced Interpretation of Trenches and Active Fault Scarps in Spain and Italy 

John Jairo Gallego Montoya, María Ortuño, Lucilla Benedetti, Moritz Kirsch, Samuel Thiele, David Garcia-Sellés, Magali Riesner, Eduardo García-Meléndez, and Marc Ollé-López

Paleoseismology extends earthquake records by documenting geological evidence of past surface-rupturing events, providing constraints for seismic source characterization, and improving the understanding of fault behavior. The reliability of paleoseismological interpretations depends on observational data and analytical methods. Conventional trenching and bedrock-scarp studies face uncertainties, as surface processes can obscure subtle deformation, and chronological correlations between units are often poorly constrained. Ground-based remote and direct sensing techniques now enable centimeter-scale multi-sensor datasets that significantly enhance observation and documentation of paleoseismic evidence.

This study builds on established methodologies to explore the integration of ground-based hyperspectral imaging, LiDAR, photogrammetry, and direct field measurements for improved detection of coseismic deformation, paleoearthquake identification, and 2D–3D reconstructions of fault displacement (for slip-rate estimation). The approach is applied to two active tectonic settings in the western Mediterranean: the Alhama de Murcia Fault within the Eastern Betics (SE Spain), with dominant transpression, and the Southern Fucino Fault System, Central Apennines (Italy), with dominant extension. At first, paleoseismological trenches were studied in alluvial sediments at the Saltador site. Second, an exhumed limestone fault scarp was analyzed at the San Sebastiano site.

At the Saltador site, 13 wall trenches excavated parallel and perpendicular to the fault, together with a natural outcrop, were logged using conventional paleoseismology and combined with remote sensing to reconstruct 2D–3D fault deformation and identify displaced alluvial-channel piercing points for slip-rate estimation. At San Sebastiano, LiDAR and photogrammetric data were combined with direct field measurements (spectroradiometry and Schmidt hammer rebound values) to characterize fault-surface roughness, mineralogical variability, and rock mass properties, to detect progressive scarp exhumation, building on existing 36Cl cosmogenic constraints. Hyperspectral imagery was acquired using an AISA Fenix 1K (400–2500 nm) at the Saltador and SPECIM FX10/FX17 (400–1700 nm) at San Sebastiano. Radiometric correction, co-registration with point clouds, and illumination modeling were performed using the hylite package. Subsequent processing included dimensionality reduction (MNF, PCA) and mineral-sensitive band ratios for lithological and structural discrimination.

The integration of hyperspectral data enhanced paleoseismological interpretations in both study areas by reducing uncertainties in coseismic deformation and surface rupture detection. At the Saltador site, previously unrecognized secondary faults and surface ruptures within alluvial sediments were revealed. Spectral band ratios improved the discrimination of sedimentary facies and erosional contacts, strengthening the identification of piercing points and deformation patterns. At least three paleoearthquake events over the past ~34 ka were confirmed, enabling refined 3D reconstructions of offset deposits and an estimated horizontal slip rate of ~0.2 mm/yr for the studied fault branch.

At San Sebastiano, visible to near-infrared hyperspectral data captured spatial variability in alteration minerals (e.g., hematite–goethite and, possibly, hydrated clay minerals), delineating vertical spectral zones that correspond to 36Cl-dated exhumation clusters, suggesting a link between mineralogical variability and progressive scarp exhumation. Combined with roughness and rock-strength measurements, these results could help to refine scarp exhumation rates, surface-rupturing earthquake sequences, and spatial variability in fault-rock exposure.

Overall, hyperspectral and multi-sensor ground-based techniques can enhance the reliability, reproducibility, and robustness of paleoseismological analyses in complex tectonic settings.

How to cite: Gallego Montoya, J. J., Ortuño, M., Benedetti, L., Kirsch, M., Thiele, S., Garcia-Sellés, D., Riesner, M., García-Meléndez, E., and Ollé-López, M.: Advancing Paleoseismology with Integrated Hyperspectral and Multi-Sensor Approaches: Enhanced Interpretation of Trenches and Active Fault Scarps in Spain and Italy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19397, https://doi.org/10.5194/egusphere-egu26-19397, 2026.

EGU26-19444 | Orals | TS3.2

 The Dual Role of Low-Plasticity Fines in the Cyclic Behaviour of Sand–Clay Mixtures 

Vedran Jagodnik, Kamil Bekir Afacan, James Leak, and Davor Marušić

Understanding how sand–fines mixtures respond cyclically is crucial for assessing liquefaction risks and how soil stiffness decreases under seismic forces. Fines, especially low-plasticity clays, greatly influence the buildup of excess pore pressure and strain during cyclic loading. However, their mechanical role at moderate fines levels is not yet fully understood.

This study presents findings from a series of stress-controlled undrained cyclic triaxial tests performed on clean sand and sand–clay mixtures. The base material consisted of a uniformly graded sand combined with low-plasticity kaolinite clay, with fines content of 10% and 15% by dry weight. In order to accurately determine the full role of fines content on the mechanical response, grading entropy coordinates where calculated for each mixture.

Cyclic loading involved applying a sinusoidal deviator stress of constant amplitude under undrained conditions. Throughout the tests, axial strain development and excess pore pressure were continuously monitored. Liquefaction was identified using two complementary criteria: (i) initial liquefaction, indicated by the complete loss of effective stress caused by excess pore pressure, and (ii) strain-based criteria, which relied on different double-amplitude axial strain thresholds.

The results demonstrate that higher fines content slows the development of excess pore pressure and delays the onset of liquefaction compared to clean sand. Both sand–clay mixtures showed less strain accumulation during initial cyclic loading, due to changes in pore space compressibility and drainage caused by low-plasticity clay. Nevertheless, at higher strain levels, significant cyclic softening, notable stiffness loss, and increased residual pore pressures were observed.

The findings emphasise the dual role of low-plasticity fines: moderate fines levels can improve cyclic resistance, while higher fines contents may weaken the granular framework and hinder effective stress transfer. The study underscores the importance of detailed analysis of void ratio and soil structure for accurately assessing the cyclic behaviour and liquefaction potential of sand–fines mixtures.

How to cite: Jagodnik, V., Bekir Afacan, K., Leak, J., and Marušić, D.:  The Dual Role of Low-Plasticity Fines in the Cyclic Behaviour of Sand–Clay Mixtures, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19444, https://doi.org/10.5194/egusphere-egu26-19444, 2026.

EGU26-19479 | ECS | Orals | TS3.2

Seismic imaging in the laboratory: Reframing fault stability using elastic-wave observables 

Michele De Solda, Giacomo Mastella, Michele Mauro, Giovanni Guglielmi, and Marco Maria Scuderi

A growing body of geophysical observations, numerical simulations, and theoretical studies indicates that the evolution of the internal structure of fault zones strongly influences fault slip behavior. However, the theoretical frameworks most commonly used to describe fault stability—such as rate-and-state friction—were originally formulated to represent frictional sliding at idealized laboratory interfaces, in which the fault is treated as an effectively two-dimensional boundary with implicitly prescribed contact-scale processes. As a result, these models do not explicitly account for the space–time evolution of fault-zone structure, including damage, granular reorganization, and fluid-mediated processes. Moreover, the state variables used to represent contact evolution are phenomenological and are only weakly constrained by seismological observations, limiting the ability of these formulations to be rigorously applied across spatial and temporal scales.

Here, we propose an experimentally derived theoretical framework that reformulates fault stability in terms of internal variables directly linked to elastic-wave observables. Using double direct shear experiments on gouge layers under controlled boundary conditions, we combine mechanical measurements with active ultrasonic probing. Full waveform inversion is employed to reconstruct one-dimensional profiles of shear modulus and attenuation across the entire sample during normal and shear loading, stable sliding, and stick–slip events.

Ultrasonic waves induce only a small perturbation in strain and therefore probe the linearized constitutive response of the system without modifying its internal state. In this context, effective elastic stiffness and attenuation can be treated as internal variables that encode the evolving fabric and organization of the fault zone. The inverted profiles reveal spatially localized regions within the gouge where elastic properties evolve during slip instabilities, enabling a data-driven identification of the dynamically active fault region, distinct from the mechanically inactive surrounding material.

Based on these observations, we reframe the classical stiffness competition problem that defines the criteria for slip instability entirely in terms of observable quantities. Specifically, we propose to substitute the phenomenological state variable with the retrieved effective viscoelastic properties. Because elastic wave propagation obeys the same governing equations across laboratory and geophysical scales, this framework provides a physically grounded pathway for connecting laboratory experiments, numerical models, and seismological imaging of natural faults. More broadly, it represents a step toward a theory of fault mechanics grounded in seismological observables and geologically relevant fault-zone structures.

How to cite: De Solda, M., Mastella, G., Mauro, M., Guglielmi, G., and Scuderi, M. M.: Seismic imaging in the laboratory: Reframing fault stability using elastic-wave observables, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19479, https://doi.org/10.5194/egusphere-egu26-19479, 2026.

EGU26-19796 | ECS | Orals | TS3.2

Multi-segmented rupture, coseismically-triggered aseismic slip, and shallow rake rotation during the 2025 Mw 7.1 Tingri, South Tibet, earthquake 

Mathilde Marchandon, Yohai Magen, James Hollingsworth, and Alice-Agnes Gabriel

On January 5, 2025, the Mw 7.0 Tingri earthquake ruptured the Dingmuco fault in the Xainza-Dinggye rift, Southern Tibet. This event was the largest normal-faulting earthquake recorded in the slowly deforming Southern Tibetan rift system and is among the largest continental normal-faulting earthquakes worldwide. Understanding the mechanics of the Tingri earthquake provides a unique opportunity to understand the regional tectonics and the rupture processes of large continental normal-faulting earthquakes in evolving rift systems. 

Here, we combine space geodetic analysis and 3D dynamic rupture simulations to investigate the earthquake. Our geodetic analysis, based on near-fault 3D optical displacement measurements and a joint optical-InSAR-SAR fault slip inversion, indicates oblique normal-left-lateral slip on a west-dipping fault that steepens toward the surface, with an average slip of 1.8 m and a shallow slip deficit of 60%. Both our fault zone width estimates and our geodetic slip model show an increase in slip-obliquity toward the surface, with left-lateral slip reaching the surface more efficiently than dip-slip, a pattern consistent with shallow rake rotation. Our geodetic analysis also reveals 0.5 m of shallow normal slip on a secondary antithetic fault located 20 km west of the main fault, which did not host aftershocks.

Next, we perform 3D dynamic rupture simulations with the open-source software SeisSol, incorporating geodetically constrained main and antithetic fault geometries, heterogeneous initial stress and fast velocity-weakening rate-and-state friction. A preferred dynamic rupture scenario that reproduces the observations suggests pulse-like, subshear rupture, with a modeled average stress drop of 6.3 MPa, higher than the observationally inferred average for normal faulting earthquakes.  A strong velocity-weakening behavior at depth, characterized by a large negative stability parameter (a − b) = −0.009, transitioning to velocity-strengthening behavior in the shallowest ~2 km is required to reproduce the observed slip distribution and moment rate release. None of our dynamic rupture scenarios dynamically triggers slip on the antithetic fault. The maximum positive dynamic and static  stress changes due to rupture on the main fault occur at shallow depths of the antithetic fault, where it is expected to be governed by velocity-strengthening friction. Together with the shallow geodetically inferred slip and the absence of aftershocks, these results indicate that slip on the antithetic fault might have occurred aseismically. However, future events across the same fault system may involve deeper coseismic slip on both faults. The high stress drop and large shallow slip deficit are characteristics of rupture on an immature fault such as the Dingmuco fault. Our study demonstrates that combining geodetic analysis with dynamic rupture simulations can shed light on  the physical processes governing seismic and aseismic slip in continental rift systems. 

How to cite: Marchandon, M., Magen, Y., Hollingsworth, J., and Gabriel, A.-A.: Multi-segmented rupture, coseismically-triggered aseismic slip, and shallow rake rotation during the 2025 Mw 7.1 Tingri, South Tibet, earthquake, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19796, https://doi.org/10.5194/egusphere-egu26-19796, 2026.

EGU26-19962 | Posters on site | TS3.2

Surface rupture characteristics and macroseismic effects of the 2025 Mw 7.7 Sagaing fault earthquake in central Myanmar 

Lin Thu Aung, Soe Min, Khaing Nyein Htay, Toe Naing Mann, Chit San Maung, Htin Aung Kyaw, Aung Kyaw, Sang-Ho Yun, and Aron J. Meltzner

The 2025 M 7.7 Myanmar earthquake affected over 30 million people across Myanmar and the broader Asian region. The earthquake caused over 5,000 fatalities, injured thousands, and left several hundred people missing. Damage extended across Myanmar, Thailand, and China, with strong shaking felt throughout Southeast Asia. The rupture propagated for over 450 km, one of the longest strike-slip earthquake ruptures worldwide, cutting through densely populated and economically important regions of central Myanmar. However, the ongoing military coup and subsequent civil conflict between the central army and People’s Defence Forces (PDFs) severely limited rescue operations and ground-based field investigations. As a result, the assessment of rupture characteristics and, slip distribution, remains limited due to gaps in ground observations.

In this study, we investigate rupture characteristics and coseismic offsets using ground-based field survey data integrated with remote-sensing observations and social media-derived felt reports and rupture information. Near the northern rupture termination, which coincides with an active conflict area, we mapped rupture patterns using newly updated Google Earth imagery, validated through reports of rupture posted by locals on social media (Facebook). Along the inferred 1839 M7+ rupture segment, details of the surface rupture were documented using unmanned aerial vehicle (UAV) and tape-and-compass surveys. In the restricted regions controlled by the central army, from Nay Pyi Taw to the southern rupture termination, coseismic offsets were measured using tape-and-compass methods only.

Slip amounts measured from ground-based surveys south of Mandalay systematically underestimate offsets determined from remote sensing, suggesting a significant fraction of the deformation occurred beyond a few meters of the main fault zone. Nonetheless, our mapping indicates that the 2025 surface rupture partially or fully overlapped multiple earlier historical Sagaing fault ruptures, including those in 1839 (Mw 7+), 1956 (Mw 7.1), 1929 (Mw ~7.0), 1930 (Mw 7.3) and 2012 (Mw 6.8). The observed macroseismic effects are comparable to those inferred for the 1839 Ava earthquake, which was poorly understood due to limited historical data. These ground-based data provide critical insights into the rupture behaviour over multiple earthquake cycles of fault segments that, at least in 2025, are inferred to have produced supershear rupture.

How to cite: Aung, L. T., Min, S., Htay, K. N., Mann, T. N., Maung, C. S., Kyaw, H. A., Kyaw, A., Yun, S.-H., and Meltzner, A. J.: Surface rupture characteristics and macroseismic effects of the 2025 Mw 7.7 Sagaing fault earthquake in central Myanmar, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19962, https://doi.org/10.5194/egusphere-egu26-19962, 2026.

EGU26-20257 | ECS | Posters on site | TS3.2

Rupture Jumping Across Fault Stepovers: An Extension of Rupture-Tip Theory of Elongated Earthquakes 

Vincent van der Heiden, Huihui Weng, Jean-Paul Ampuero, and Ylona van Dinther

Stepovers between fault segments are a key structural control on rupture propagation, often determining whether ruptures terminate or cascade into large, multi-segment earthquakes. These dynamics critically influence earthquake magnitude and seismic hazard. Theoretical models, in particular the rupture-tip equation of motion for elongated ruptures (Weng & Ampuero, 2019), describe rupture growth along planar faults of finite widths. However, they do not account for the potential of rupture jumping across geometric discontinuities or frictional barriers. In this study, we use 2.5D dynamic rupture simulations with the spectral element method (SEM2DPACK software) to determine how the critical distance Hc for rupture jumping across stepovers in elongated fault systems of two parallel normal faults depends on prestress level S’ and seismogenic width W (Fig. a). We simulate dynamic rupture on a primary fault and record the resulting stress perturbations on a locked secondary fault. The critical stepover distance Hc​ is determined by computing the strength excess required for Coulomb failure on the secondary fault over a static process zone Lc. This approach is validated by complete dynamic rupture simulations in a selected set of fault stepover cases. For two co-planar faults we find a Hc/W ~ 1/S’n scaling relationship with n=2 for short Hc (near-field) and n=1/2 for large Hc (far-field) (Fig. b), consistent with dynamic nucleation thresholds with stepovers. For non-co-planar faults we find a Hc/W ~ 1/S’n scaling relationship with n=1 for near-field transitioning to n=2 for far-field (Fig. c). This transition is governed by the angular dependence of the stopping phase emitted by rupture arrest on the primary fault and the resulting dynamic trigger. These scaling relationships for co-planar and non-co-planar faults will be incorporated into the rupture-tip equation of motion, extending its applicability to segmented fault systems. The updated framework will improve assessment of rupture potential in complex fault networks, such as the 2023 Kahramanmaraş sequence (strike-slip), the 2010 Maule earthquake (subduction zone), and the 2016 Kaikōura earthquake (multifault rupture), as well as for induced earthquakes (e.g., the Groningen gas field). Particularly, extrapolating our results suggests that faults with small W need to be highly critically stressed to jump over even short distances (e.g., >94% stressed to jump over 300 m in Groningen’s 300 m wide gas reservoir). Since fault slip is expected to occur locally before reaching such high averaged stresses, this implies that rupture jumping in induced seismicity settings with small W is highly unlikely. These findings contribute to a unified theory of rupture propagation incorporating complex segmented systems.

How to cite: van der Heiden, V., Weng, H., Ampuero, J.-P., and van Dinther, Y.: Rupture Jumping Across Fault Stepovers: An Extension of Rupture-Tip Theory of Elongated Earthquakes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20257, https://doi.org/10.5194/egusphere-egu26-20257, 2026.

EGU26-20817 | Posters on site | TS3.2

Assessing the longevity and stationarity of surface velocities for seismic hazard in the central Apennines (Italy) by combining InSAR and fully dynamic earthquake cycle modeling 

Erwan Pathier, Maaike Fonteijn, Alexander Koelzer, Anne Socquet, Niek van Veenhuizen, and Ylona van Dinther

The central Apennines (Italy) are characterized by active normal faulting that is largely clustered in space and time, as documented by both historical and paleoseismic records. The 2016-2017 central Italy earthquake sequence, comprising a series of Mw 5 to Mw 6.5 events within half a year, exemplifies this behavior. Over longer timescales, 36Cl dating of Holocene fault scarps reveals earthquake clustering in the Fucino basin. Although the central Apennines have dense geodetic and seismological observations, these instrumental datasets only cover a small portion of the seismic cycle. This raises fundamental questions about how representative the present-day deformation signals are of long-term tectonic loading and seismic hazard. Here, we address the following questions: How representative is the current geodetic signal over multiple earthquake cycles in an area characterized by a dense fault network? How do surface velocities evolve through the earthquake cycle, and how does the spatial and temporal distribution of earthquakes relate to this evolution?

We combine new InSAR observations with newly developed seismo-thermo-mechanical models with an invariant rate-and-state friction (STM-RSF) and a visco-elasto-plastic rheology in a geodynamic framework. This fully dynamic earthquake cycle model resolves the inter-, post- and co-seismic periods, as well as cumulative deformation over several seismic cycles. We build on previous STM modeling in the central Apennines (Fonteijn et al., in prep). Faulting is localized on pre-defined weak zones from geology and the Fault2SHA active faults database, but can also occur outside the weak zones.

We analyzed InSAR time-series to study interseismic surface deformation in the central Apennines. We detect significant short wavelength velocity variations across faults of 0.5 to 2 mm/yr, which could possibly be explained by bookshelf faulting. Additionally, we simulated an earthquake sequence of six large normal-faulting earthquakes over ~8000 years in the central Apennines. These earthquakes occur on different normal faults in sequence before faults are reactivated, with rupture on one fault transferring stresses to adjacent faults. We also find rupture of a spontaneously arising antithetic fault and accumulated vertical displacement shows block-faulting behavior. We assess the variability of interseismic surface displacements and compare with InSAR interseismic displacements. Preliminary results show significant variations in vertical velocities in both duration and intensity over 8000 years, with alternating periods of subsidence and uplift in the orogen. This new modelling approach for the first time allows for a comparison of surface displacements over multiple earthquake cycles with short-term geodetic observations. The outcome of this study will have important implications for how to use geodetic data for seismic hazard assessment.

How to cite: Pathier, E., Fonteijn, M., Koelzer, A., Socquet, A., van Veenhuizen, N., and van Dinther, Y.: Assessing the longevity and stationarity of surface velocities for seismic hazard in the central Apennines (Italy) by combining InSAR and fully dynamic earthquake cycle modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20817, https://doi.org/10.5194/egusphere-egu26-20817, 2026.

EGU26-20840 | ECS | Posters on site | TS3.2

Improving Real-Time Earthquake Source Characterization Using Diffusion Model Based Broadband Envelope Synthetics 

Francesco Alexandr Colosimo, Dario Jozinović, and Maren Böse

Reliable real-time earthquake source characterization requires the rapid selection of solutions from competing algorithms while minimizing false alarms. To address this challenge, Jozinović et al. (2024) have proposed a ground-motion-envelope-based goodness-of-fit approach that  ranks candidate source solutions using amplitude ratios and cross-correlation between observed and predicted waveform envelopes. In its current implementation, however, this approach relies on the ground motion envelope prediction model of Cua (2005), which is limited to small-to-moderate sized  earthquakes. 

In this work, we explore the benefits and limitations of replacing this empirical model with envelopes derived from machine-learning-generated broadband (up to 50 Hz) synthetic waveforms (Palgunadi et al., 2025). These synthetics are generated using a conditional denoising diffusion model, conditioned on preliminary source parameters (magnitude, hypocentral distance, depth), and site effects. For large magnitude events, we superpose point-source synthetics to produce realistic finite-fault rupture waveforms using the  SWEET workflow (Colosimo, MSc thesis).

We find that the diffusion-based synthetics extrapolate realistically across a broader magnitude range and reproduce observed envelope characteristics as well as, or even better than, the empirical prediction model. This capability has the potential to enable  earlier and more reliable identification of correct source solutions, reduce magnitude and location bias, and improve robustness for larger events.

 

How to cite: Colosimo, F. A., Jozinović, D., and Böse, M.: Improving Real-Time Earthquake Source Characterization Using Diffusion Model Based Broadband Envelope Synthetics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20840, https://doi.org/10.5194/egusphere-egu26-20840, 2026.

EGU26-21171 | Posters on site | TS3.2

Modelling complex fault systems with the Particle Finite Element Method (P-FEM) 

Andrea Bistacchi, Matteo Ciantia, Riccardo Castellanza, Silvia Mittempergher, and Federico Agliardi

Developing numerical models of faulting in the upper crust remains a challenge due to limitations in numerical algorithms and problems in choosing realistic constitutive models. This results in strong limitations when trying to model the strain and stress fields, and elastic and plastic energy release (i.e. stress times strain), under realistic parametrization obtained from lab experiments, particularly regarding mechanical and chemical weakening that leads to localization as observed in nature.

Here we explore applications of the Geotechnical Particle Finite Element Method (P-FEM), a large-deformation numerical tool developed to capture detailed progressive failure and fracturing using a non-local formulation.

P-FEM allows modelling localized shear bands that naturally emerge independent of mesh discretization, both in thickness and orientation. Moreover, continuous remeshing in a Lagrangian framework enables modeling of large deformations, and techniques used to minimize numerical diffusion help produce realistic localized shear/fault zone patterns.

The elastoplastic constitutive models can be calibrated using multi-method lab tests (e.g. monoaxial, triaxial, Brazilian, oedometer, etc.) to include complex non-linear effects, such as strain weakening and softening, poroelasticity, strength envelopes with a cap (i.e. porosity collapse in compression), and mechano-chemical degradation. This allows for realistic simulations of geo-materials with contrasting properties, including non- or weakly-cohesive fault gouges, weak porous rocks, and stronger brittle frictional-plastic materials.

After an overview of the method, we will show how P-FEM is particularly suited for investigating deformation in the upper crust including (i) fault nucleation and growth in mechanically layered materials, (ii) the interplay between faulting and folding in thrust belts, and (iii) the development of fault damage and/or process zones in materials with heterogeneous mechanical properties.

How to cite: Bistacchi, A., Ciantia, M., Castellanza, R., Mittempergher, S., and Agliardi, F.: Modelling complex fault systems with the Particle Finite Element Method (P-FEM), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21171, https://doi.org/10.5194/egusphere-egu26-21171, 2026.

EGU26-21225 | Posters on site | TS3.2

Integrating Structural, Geomechanical, and Passive Seismic Data to Investigate Site Effects along an Active Normal Fault Zone 

Alberto Pizzi, Silvia Giallini, Maurizio Simionato, Chiara Puricelli, and Alessandro Pagliaroli

Understanding earthquake site effects in fault-controlled geological settings remains a key challenge for seismic hazard assessment, particularly in intramontane basins affected by active normal faulting. In these settings, fault-zone site effects are expected due to the abrupt contact between thick soft and/or granular sedimentary basin-fill and the carbonate bedrock, which is characterized by highly variable fracture intensity and orientation.

In this study, we present the results of a multidisciplinary investigation aimed at characterizing fault-related site effects along the Monte Morrone fault system, a major Quaternary normal fault bounding the eastern margin of the Sulmona intramontane basin (Central Apennines, Italy) and recognized as a key seismogenic structure in the region.

A passive seismic survey was conducted at three sites located along the fault zone: Eremo di Sant’Onofrio, Roccacasale North, and Roccacasale South. The two Roccacasale sites are structurally located within the fault core and damage zone of the Monte Morrone fault system, characterized by intense deformation and pervasive fracturing. Ambient noise data were acquired and processed using the Horizontal-to-Vertical Spectral Ratio (H/V) technique to investigate resonance frequencies and potential directional amplification effects. Where suitable reference conditions were identified, the data were further analyzed using the Standard Spectral Ratio (SSR) technique to provide a more robust estimate of relative amplification.

Geophysical observations were integrated with detailed structural and geomechanical field measurements. These include fault architecture mapping, fracture density and fracture orientation analysis, and in-situ rock mass characterization through Schmidt hammer rebound measurements. The combined dataset highlights significant lateral variations in seismic response between the investigated sites, which can be directly related to the features of the fault-zone structures, damage intensity, and rock mass stiffness. Directional amplification patterns observed in H/V are consistent with the dominant orientation of fault-related discontinuities, suggesting a strong structural control on local seismic response.

Our results are consistent with previous studies documenting fault-controlled site effects and directional amplification within active fault zones in the central Apennines (e.g., Pischiutta et al., 2013, Vignaroli et al., 2019), and further emphasize the role of fault-core properties and damage-zone architecture in modulating seismic ground motion. These findings support the growing evidence that structural heterogeneities within regional fault zones play a key role in controlling seismic wave propagation and site effects, even at rock sites traditionally considered mechanically homogeneous. Our results suggest that fault cores and associated damage zones should be treated as mechanically distinct domains, characterized by stiffness contrasts and velocity anisotropies capable of modifying the amplitude, frequency content, and directionality of seismic ground motion.

From an application perspective, the multidisciplinary dataset presented here provides further evidence of the importance of correctly representing fault zones in two-dimensional subsurface models for numerical simulations of local seismic response. Explicitly considering the internal architecture of faulted rock masses, rather than assuming uniform "bedrock" conditions, can significantly improve ground motion modeling and help reduce uncertainties in seismic microzonation studies in tectonically active regions.

References

Vignaroli et al., 2019 Domains of seismic noise... BEGE, doi.org/10.1007/s10064-018-1276

Pischiutta et al., 2017. Structural control on the directional.. EPSL, doi:10. 1016/j.epsl.2017.04.017

How to cite: Pizzi, A., Giallini, S., Simionato, M., Puricelli, C., and Pagliaroli, A.: Integrating Structural, Geomechanical, and Passive Seismic Data to Investigate Site Effects along an Active Normal Fault Zone, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21225, https://doi.org/10.5194/egusphere-egu26-21225, 2026.

The Yingjing-Mabian-Yanjin tectonic blet (YMYTB) serves as a critical boundary structure between the southeastern margin of the Tibet Plateau and the Sichuan Basin. Although seismicities has been frequent since the late Quaternary, the activity of individual faults within the tectonic belt remains unclear, introducing significant uncertainty in understanding and assessing the current regional crustal deformation patterns and seismic hazards. Particularly, the southern segment of the tectonic belt near the Leibo fault has experienced the 1216 Mahu M7 earthquake and several strong earthquake swarms of magnitude 6 or above. However, research on this fault zone is limited, and there is still a lack of reliable evidence to determine its most recent activity period and its relationship with nearby major earthquakes.

To address this issue, this study conducted paleoseismic trenches on the northern, central, and southern branches of the Leibo fault, based on the interpretation of high-resolution remote sensing imagery and field geological-geomorphological investigations. The following conclusions were drawn:

(1) Based on paleoseismic event identification markers, three, three, and five paleoseismic events were revealed on the three branch faults, respectively. Dating results of radiocarbon samples constrained the occurrence times of the three paleoseismic events on the northern branch fault to 21,190–20,590 BC (EP1), 20,550–12,120 BC (EP2), and after 12,090 BC (EP3). The timings of the three strong seismic activities on the central branch fault were 7,400–6,320 BC (EY1), 5,690–2,620 BC (EY2), and 2,220 BC–170 AD (EY3). The occurrence times of the five surface-rupturing seismic events on the southern branch fault were 14,660–9,300 BC (ES1), 9,270–7,560 BC (ES2), 600–640 AD (ES3), 740–1,440 AD (ES4), and 1,650–1,900 AD (ES5). The paleoseismic results indicate that all branch faults of the Leibo fault zone are Holocene active faults.

By comparing the occurrence times of paleoseismic events on each branch fault, it is determined that the Leibo fault zone has experienced at least 10 surface-rupturing paleoseismic events since the Late Pleistocene. The corresponding age ranges are 21,190–20,590 BC (E1), 14,600–9,300 BC (E2), 12,090–11,820 BC (E3), 9,270–7,560 BC (E4), 7,400–6,320 BC (E5), 5,690–2,620 BC (E6), 2,220 BC–170 AD (E7), 600–640 AD (E8), 740–1,440 AD (E9), and 1,650–1,900 AD (E10). The paleoseismic history of the Leibo fault zone reveals that the strong seismicities of the three branch faults exhibit significant spatial independence and temporal clustering, indicating that the branch faults of the Leibo fault zone are independent seismogenic structures.

(3) Based on historical earthquake records and paleoseismic research results, this study proposes that the seismogenic structure of the 1216 Mahu M7 earthquake is the southern branch of the Leibo fault. Additionally, the Leibo fault likely participated in the rupture of the 1935–1936 Mabian M6¾ earthquake swarm.

(4) By collecting and analyzing the magnitudes of strike-slip earthquake events that generated surface ruptures in western China since 1920, it is inferred that the lower limit of the magnitudes of paleoseismic events revealed on the Leibo fault zone is 6.5. Furthermore, based on the fault length and empirical relationship, it is estimated that the Leibo fault has the capability to generate earthquakes with magnitudes of 7.0 or higher.

How to cite: Sun, H.: Late Quaternary Strong Earthquake History of the Leibo Fault on the southeastern margin of the Tibetan Plateau, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21381, https://doi.org/10.5194/egusphere-egu26-21381, 2026.

EGU26-21777 | ECS | Orals | TS3.2

Structural controls on normal fault synchronization and simultaneous earthquake clustering 

Francesco Iezzi, Sgambato Claudia, Gerald Roberts, Zoe Mildon, Jenni Robertson, Joanna Faure Walker, ioannis Papanikolaou, Alessandro Maria Michetti, Sam Mitchell, Richard Shanks, Richard Phillips, Kenneth McCaffrey, and Eutizio Vittori

Slip-rate variations over multiple seismic cycles play a fundamental role in controlling the behaviour of active fault systems, as they are linked to spatio-temporal earthquake clustering and can influence the recurrence patterns of adjacent faults. However, processes that produce slip-rate fluctuations are yet to be fully defined. Despite their importance, the physical mechanisms responsible for such slip-rate fluctuations remain only partially understood. In this study, we investigate whether interactions between neighbouring along-strike brittle faults and their underlying viscous shear zones can generate slip-rate variability associated with synchronous earthquake clustering and fault system synchronization. We focus on nine normal faults and related shear zones within the Central Apennines fault system (Italy), arranged in six along-strike fault pairs characterized by different fault spacings and strike geometries. We integrate cosmogenic 36Cl dating of tectonically exhumed fault scarps with numerical modelling of differential stress transfer between interacting fault–shear-zone pairs. The results identify a mechanism capable of producing simultaneous earthquake clusters, driven by the synchronization of high driving stresses within the viscous shear zones beneath the brittle faults. This behaviour is strongly modulated by along-strike fault spacing and strike variations. In settings with closely spaced fault pairs and limited strike variations, earthquake clusters induce positive differential stress variations on neighbouring shear-zones of sufficient magnitude to induce positive slip-rate variations on their overlying brittle faults. This produces positive feedback mechanism that sustains the occurrence of earthquake clusters that will continue to positively load the neighbouring shear zones. These findings provide new insights into fault system dynamics across multiple timescales and have important implications for seismic hazard evaluation.

How to cite: Iezzi, F., Claudia, S., Roberts, G., Mildon, Z., Robertson, J., Faure Walker, J., Papanikolaou, I., Michetti, A. M., Mitchell, S., Shanks, R., Phillips, R., McCaffrey, K., and Vittori, E.: Structural controls on normal fault synchronization and simultaneous earthquake clustering, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21777, https://doi.org/10.5194/egusphere-egu26-21777, 2026.

EGU26-22278 | ECS | Orals | TS3.2

One Big Earthquake or Many? Fault Segmentation in the Eastern Precordillera, western Argentina 

Shreya Arora, Drew Cochran, Erik Janson, Gustavo Federico Ortiz, Jeremy Rimando, Nathan Brown, Melina Villalobos, Raul Gomez, and Yann Klinger

Why do some earthquakes repeatedly rupture discrete fault segments, while others rupture entire

faults? Answering this remains fundamental to improving seismic hazard analysis and, in turn, to

hazard preparedness and mitigation efforts. Over the past two decades, several mechanisms for

rupture termination and propagation have been proposed, including variation in geometric,

structural, and geologic characteristics of faults (Aki, 1979; King and Nabelek, 1985). In this study

we investigated the Eastern Precordillera (EPC) of the Andes Mountain in Argentina which is

classified into three segments: Villicum, Las Tapias, and Zonda–Pedernal (Siame et al., 2002) to

determine whether the historical surface ruptures associated with major earthquakes crossed the

segment boundaries, or whether rupture propagation was arrested by structural asperities

indicating an asperity-controlled behavior. To address this, we conducted a new paleoseismic

investigation at this site to complement and integrated with the preexisting dataset to evaluate the

extent of past surface ruptures in relation to fault geometry and structural segmentation. We have

complied earthquake timing of six earthquakes. Preliminary results suggest that, of the six

identified events, only one earthquake appears to have ruptured across an ~18 km-long segment

gap, including a ~4 km stepover and notable lithologic variation evidence consistent with a multi-

segment rupture event.

How to cite: Arora, S., Cochran, D., Janson, E., Ortiz, G. F., Rimando, J., Brown, N., Villalobos, M., Gomez, R., and Klinger, Y.: One Big Earthquake or Many? Fault Segmentation in the Eastern Precordillera, western Argentina, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22278, https://doi.org/10.5194/egusphere-egu26-22278, 2026.

EGU26-23007 | Posters on site | TS3.2

Interseismic Slip Rates of the Sındırgı Fault Forecast Extensional Kinematics During the 2025 M6+ Earthquakes 

Sevil Cansu Yavuz, Rahmi Nurhan Çelik, and Fatih Bulut

We investigated the geometry and the kinematics of the Sındırgı fault, which was activated during the two M6+ earthquakes (10.08.2025 and 27.10.2025) and their aftershocks. We analyzed all available seismographs from KOERI (Kandilli Observatory and Earthquake Research Institute) and AFAD (Disaster and Emergency Management Authority) to identify fault geometry, earthquake locations, and focal mechanisms. We analyzed P-wave initial polarities and arrival times of a total of 43 M4+ earthquakes including two mainshocks (waveforms from KOERI and AFAD). Fault plane solutions as well as the accurate hypocenter locations indicate that the majority of the mainshocks and the aftershocks activated a south dipping fault. The results indicate an average strike of 110 ± 5.6°, a dip of 61.6 ± 4.4°, and rake a rake -124.6 ± 2.3°. Additionally, we investigated inter-seismic slip rates using 2D dislocation model analyzing the GNSS velocity field. We transformed the most recent velocity field into Anatolian-fixed reference frame. We decomposed GNSS velocities into fault-parallel and fault-perpendicular components and applied 2D arctan curve fitting to simultaneously determine the slip rates and the fault locking depths. Bootstrap error analysis was performed (1σ) to assess error bounds. The lateral motion is nearly negligibly small; however, fault-perpendicular velocities indicate the extension along the Sındırgı fault at 2.34 ± 0.69 mm/y slip rate. Inter-seismic slip rates suggest a rake of -95.2°, a nearly pure normal fault, which is consistent with average mainshock-aftershock rakes. In this context, GNSS-derived interseismic slip rates are capable of forecasting the extensional kinematics of the Sındırgı fault that generated two predominantly normal-faulting M 6+ earthquakes in 2025.

How to cite: Yavuz, S. C., Çelik, R. N., and Bulut, F.: Interseismic Slip Rates of the Sındırgı Fault Forecast Extensional Kinematics During the 2025 M6+ Earthquakes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-23007, https://doi.org/10.5194/egusphere-egu26-23007, 2026.

EGU26-2868 | Orals | TS1.5

Changes in fluid migration in ductile shear zones during tectonic switching may explain the formation of hydrothermal ore deposits 

Melanie Finch, Ben Knight, Andy Tomkins, Enrique Gomez-Rivas, Paul Bons, Bruno Ribeiro, and Alanis Olesch-Byrne

A common feature of many hydrothermal ore deposits is that they formed during tectonic switches between extension and shortening on plate boundaries. Several theories to explain this relationship have been proposed but evidence for a mechanism remains elusive. Many of these ore deposits occur within or adjacent to ductile shear zones that changed movement direction during the tectonic switch. Prior to tectonic switches, shear zone structures evolve to orientations optimised to accommodate deformation, which maximises strain rate and creates permeable pathways for fluid migration. But when a tectonic switch occurs the structures are misoriented and must reconfigure to accommodate the new shearing direction. Using numerical models of shear zone evolution, we determined that during tectonic switches the microstructural reconfiguration reduces the strain rate and mean stress, causing fluid influx into the shear zone. To further explore the effect of this microstructural reconfiguration on fluid migration we examined rocks of the Bergen Arc shear zone in Norway in a transition zone where sinistral shearing is progressively overprinted by dextral shearing. We find that during the tectonic switch, accretionary veins of quartz, ankerite and calcite formed in dilatational spaces that opened as the sinistral structures were reconfigured to accommodate dextral shearing. With increasing strain, fluid migration into the shear zone became more pervasive, evidenced by larger vein networks and hydrothermal breccias. Coincident with vein formation there is a statistically significant increase in the water content in quartz as determined by synchrotron FTIR. These data indicate that the microstructural reconfiguration in shear zones during tectonic switching causes fluid influx into shear zones. This process may be responsible for the introduction of ore fluids into the shear zone and the formation of hydrothermal ore deposits during tectonic switching.

How to cite: Finch, M., Knight, B., Tomkins, A., Gomez-Rivas, E., Bons, P., Ribeiro, B., and Olesch-Byrne, A.: Changes in fluid migration in ductile shear zones during tectonic switching may explain the formation of hydrothermal ore deposits, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2868, https://doi.org/10.5194/egusphere-egu26-2868, 2026.

EGU26-5095 | Posters on site | TS1.5

Alteration pathways in Cenozoic volcanic suites of the Styrian Basin: an integrated petrographic–geochemical approach  

Veronika Tenczer, Christoph von Hagke, Mathias Hopfinger, Anja, C. Hörger, Ena Topalović, and Inga Strähler

We present a study that investigates the post-eruptive geochemical evolution of six sites from Miocene and Pliocene volcanic suites from Styria (SE Austria). The sites are Weitendorf, Gleichenberg, Klöch, Hochstraden, Steinberg and Fürstenfeld. We focus on a stratigraphic sequence that transitions from lavas to porous, laminated ash tuffs and pyroclastic rocks. An integrated approach was performed combining petrography, whole rock geochemistry, and isocon–τ relative mass balance modeling to decipher fluid–rock interaction and element mobility. 

Detailed petrography (based on microscopy work with thin sections) show that the six sites exhibit different alteration stages ranging from weak alteration over mafic phenocryst alteration (reducing versus oxidizing) to palagonite and zeolite formation. Mass balance modeling allows us to establish alteration pathways where Miocene units follow a path of pronounced alkali leaching and Mn depletion, whereas Pliocene high‑alkaline units display more variable pathways. 

The site‑specific fingerprints delineate contrasting nutrient and redox landscapes that provide a geochemical baseline for further studies on soil development and vegetation. 

How to cite: Tenczer, V., von Hagke, C., Hopfinger, M., Hörger, A. C., Topalović, E., and Strähler, I.: Alteration pathways in Cenozoic volcanic suites of the Styrian Basin: an integrated petrographic–geochemical approach , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5095, https://doi.org/10.5194/egusphere-egu26-5095, 2026.

Significant breakthroughs have been made recently in petroleum exploration within ultra-deep (burial depth > 6,000 m) carbonates in the Tarim Basin, northwestern China. The discovery of several large-scale oil and gas accumulation (e.g., Shunbei and Fuman) in these deeply buried, highly fractured and vuggy carbonates highlights the crucial role of strike-slip faults in reservoir development. However, the formation mechanisms of these ultra-deep, fault-controlled carbonate reservoirs remain poorly understood. It is therefore essential to conduct experimental simulations investigating the controlling factors and evolutionary trends governing the impact of deep CO₂-rich fluids on carbonate rocks.

For this reason, experiments were performed by using an ultra-deep, multi-tectonic-stage, high-temperature and high-pressure reservoir simulation system. This study focused on two key aspects, the dissolution mechanisms of dolomite in CO₂-saturated solutions, and the evolutionary trends of pore structure in carbonate rocks with different initial pore types during dissolution. Overall, two major findings were obtained. First, within temperature of 40–220 °C and pressure of 10–132 MPa, the saturated dissolution capacity of dolomite in CO₂-rich fluids exhibited an initial increase that was followed by a decrease, with the maximum dissolution occurred approximately at 60–110°C. This provides the theoretical basis for predicting favorable depth intervals where large-scale secondary pores may be formed in dolomite by deep CO₂-rich fluids. Second, influenced by the deep CO2-rich fluid dissolution, both pore-dominated and fracture-dominated limestones tend to transform into fracture-vug reservoirs. Dissolution preferentially occurred along major fractures, gradually enhancing reservoir space and percolation capacity, ultimately becoming concentrated within these main fracture systems.

These results led to the construction of a genetic model for the development of fault-controlled, fracture-vug carbonate reservoirs. When deep CO2-rich fluid activity coincides with fault development periods, fluids preferentially migrate into main faults, leading to dissolution-enlarged porosity along fault planes. When fluids migrate to fault intersections, they stagnate and induce dissolution and connectivity to form vugs. The fluids continue to expand along multiple sets of pre-existing faults, stagnating at new fault intersections to create more vugs. Such dissolution cycles are controlled by the episodic regional tectono-fluid activity. Ultimately, early-formed fracture-vug systems may become merged to formwell-connected fracture-vug reservoirs with superior reservoir performance. This model effectively explains the differences in dissolution and modification effects observed in different segments of strike-slip faults and clarifies the underlying mechanisms.

How to cite: She, M., Qiao, Z., and Liu, Y.: Influence of Deep CO₂-Charged Fluids on the Development of Carbonate Reservoirs in Fault-Controlled, Ultra-Deep burial setting: Insights from Water-Rock Interaction Experiment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6340, https://doi.org/10.5194/egusphere-egu26-6340, 2026.

Deep fluid activities driven by strike-slip fault movement play important roles in the modification of carbonate and hydrocarbon accumulation. The complexities of deep fluid sources and temperature-pressure variations during strike-slip fault movement complicate fluid-rock reactions, diagenetic modification processes and the formation and evolution of reservoirs in deep to ultradeep carbonate strata. To understand the temporal-spatial coupling between strike-slip movement and deep fluid migration, we investigate the migration periods and sources of deep fluids along strike-slip fault belts in the Fuman Area of the Tarim Basin, considering the geometry of the strike-slip faults and analysing laser ablation U-Pb dating, clumped isotopes, REE, and fluid inclusions in diagenetic products such as calcite, chert, and quartz.

U-Pb age results indicate that vug-filling calcites were emplaced between 460.8 ± 3.4 and 448.6 ± 5.3 Ma, and at 335 ± 19 Ma during the early Hercynian orogeny, while the fracture-filling and megacrystalline calcites formed between 364 ± 53 and 282.9 ± 5.4 Ma, and during periods from 324 ± 23 to 300.9 ± 4.8 Ma and from 244.13 ± 13 to 240.5 ± 4.1 Ma, respectively. The latest fracture-filling calcites show a slightly younger U-Pb age of ca. 158 ± 17 Ma. In addition, the U-Pb ages for the chert and quartz in fractures (459 ± 57 Ma, 252 ± 56 Ma, and 174 ± 35 Ma) fall within the middle Caledonian, late Hercynian, and Yanshanian periods.

The combination of geochemical analyses on calcites, including clumped isotopes, d13C, d18O, and 87Sr/86Sr isotopes, REE, and fluid d18O calculation, suggests that these calcites were precipitated from formation fluids mostly of meteoric water origin with some input from hydrothermal fluids. Hydrothermal fluid flow resulted from strike-slip fault activity and volcanism, whereas meteoric water intruded from uplifted areas along the faults during tectonic quiescence. This study shows that the formation of fracture-related cavern reservoirs in the Fuman oil field is related to the early Hercynian, late Hercynian, and Yanshanian tectonic events and their associated fluid activity. The methodologies and outcomes of the present study may guide future hydrocarbon exploration in the Tarim Basin and be applied to other oil fields with similar tectonic backgrounds.

How to cite: Qiao, Z.: Fluid activities Controlled by Intra-craton Strike-slip Faults: A Case Study of Ordovician in Fuman Area in Tarim Basin, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6851, https://doi.org/10.5194/egusphere-egu26-6851, 2026.

Abstract

The volcanic rocks of the Mesoproterozoic Xiong’er Group (Changcheng System) in the Ordos Basin are pervasively albitized, a phenomenon mainly attributed to lava-seawater interaction. Understanding the mineralogical and textural imprints of this alteration is therefore essential.

This study focuses on deep core samples of the Xiong’er Group from the southwestern Ordos Basin. An integrated methodology was applied, combining petrographic observation with geochemical analyses (major and trace elements, TIMA automated mineralogy, C-O isotopes, and zircon U-Pb dating). Our results confirm intense lava-seawater alteration in the Xiong’er Group magmas and define the diagnostic mineral assemblages and textures produced by this process. Additionally, a comparative analysis with coeval volcanic rocks from the eastern Ordos Basin was conducted to reconstruct the tectonic environment during magma genesis.

Key findings are summarized as follows:

(1) Core and thin-section observations reveal volcanic rocks with vesicular-amygdaloidal textures, plagioclase-phyric porphyritic structures, and interbedded sedimentary layers. Distinct dark-reddish alteration zones occur along lithological contacts. Microscopically, the rocks show porphyritic texture with feldspar phenocrysts in a cryptocrystalline groundmass. Vesicles are commonly filled with calcite, quartz and chlorite.

(2) Geochemical data indicate that the Xiong’er Group volcanic rocks in the southwest basin are predominantly basaltic. They exhibit high alkalinity (σ = 4.6~10.6) alongside anomalous silica contents, classifying them as basic to intermediate igneous rocks. Rare earth element patterns are consistent with an intracontinental rift setting linked to mantle plume activity, with evidence of crustal contamination.

(3) TIMA automated mineralogical mapping shows that feldspar phenocrysts in the basalts are exclusively albite. The groundmass is pervasively altered by chloritization and argillization. Slilceous sediments occur widely, filling vesicles in basalts and appearing within sedimentary rocks at basaltic contacts.

(4) Marked petrological and geochemical differences exist between the Xiong’er Group volcanic rocks in the southwest and eastern Ordos Basin, reflecting contrasting tectono-magmatic environments-intracontinental rift versus continental arc settings.

The results advance the understanding of mineral alteration and element exchange during such interactions at the micro-scale and provide key mineralogical constraints on lava-seawater alteration processes.

Keywords

Xiong’er Group, Volcanic Rocks, Lava-Seawater Interaction, Alteration Mineralogy, Geochemistry, Ordos Basin

How to cite: Ren, Y. and Chen, Z.: Lava-Seawater Interaction of the Mesoproterozoic Xiong’er Group Volcanic Rocks in the Southwestern Ordos Basin: Insights from Alteration Mineralogy and Geochemistry, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7121, https://doi.org/10.5194/egusphere-egu26-7121, 2026.

Geological fluids play crucial roles in the stabilisation of minerals and in the mobilization and redistribution of elements during mid- to lower-crustal metamorphism, thereby influencing the chemical evolution of continental crust. The current study demonstrates extensive fluid-induced alterations and formation of a highly peraluminous (A/CNK~30), ferromagnesian yet silica-calcium and alkali-poor rock from the Makrohar granulite belt, part of the Proterozoic mobile belt, Central Indian Tectonic Zone. The study demonstrates a black, garnet-rich, massive rock composed of garnet, cordierite, sillimanite, quartz, and ilmenite, lacking gneissic banding and intruded by multiple veins in the outcrop. Thin microscopic veinlets consist of biotite (80% modal volume) with smaller proportions of quartz±cordierite and fibrolites. Late-stage veins of variable thickness, evident from the outcrop scale, contain coarse-grained sillimanite-quartz-garnet, with large sillimanite grains growing at high angles to the vein boundary, indicating a syntaxial growth. Vein garnets frequently grow inward from the vein wall, often growing on older garnet in the host. Phase equilibrium modelling, coupled with conventional thermobarometry, constrains the P-T conditions of the stabilization of the host rock at approximately 600ºC and 5 kbar. Slightly magnesian cores of the host garnet (XMg) yield marginally higher temperatures (~680ºC) than the rim (garnet isopleth yielding ~580ºC).

Garnet grains in the host rock display a distinct positive europium anomaly (Eu/Eu*), likely resulting from garnet growth in the absence of plagioclase. A moderate Gd/Dy ratio in the host garnet indicates stabilization at approximately 4 kbar, supporting low-pressure estimates from conventional barometry and phase-equilibria modelling. Rim-to-rim trace element profiles along host garnet grains show a uniform distribution of Sc, Y, and HREEs in the core, with oscillations and a sharp increase near the rim, suggesting that reverse zoning in HREEs was likely caused by homogenization by intragranular diffusion in the core but remained largely unaffected towards the rim. Whole-rock chemistry of the host, feldspar-free high-variance mineralogy, absence of leucosome and reverse zoning of Y-HREE, positive Eu/Eu* within garnet indicate potential metasomatic alteration of the host itself.

Garnets within the quartz-sillimanite veins exhibit distinct oscillations in trace element concentrations along wall-to-wall line scans, indicating minimal effects of diffusion and grain growth in the presence of vein-fluid. Ca and Mn zoning within vein garnet exactly replicate each other with gradual increase from vein-wall to vein-axis regions of the grains. Y and HREEs show resonating patterns with sharp central peaks in the mid-axis and oscillatory zoning within the vein-wall garnet portions. Sc and MREEs, i.e., Sm, Eu, Gd, Tb still show central peaks along with an annular maxima added with the oscillation within the vein-wall garnets. REE mobilization, at least in micro-scale, is further evident from large monazite clusters observed in sillimanite-quartz-garnet veins. The presence of large sillimanite grains further demonstrates the fluid's capacity to transport aluminium. The absence of any hydrous phases in the vein supports the prevalence of low-H2O-bearing fluid. XCO2-µK2O and µK2O-µFeO topology further confirms that the intrusion of low-H2O fluid presumably destabilized the host biotite, producing garnet and quartz in the vein.

How to cite: Chakrabarty, A., Anczkiewicz, R., and Sanyal, S.: Fluid-induced redistribution of REEs within alumino-silicate veins and peraluminous host rock in the Central Indian Tectonic Zone, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7449, https://doi.org/10.5194/egusphere-egu26-7449, 2026.

EGU26-7493 | ECS | Orals | TS1.5

How hard do crystals push when growing under confinement? Real-time measurements of surface forces during hydration of periclase to brucite 

Viktoria Trautner, Melania Rogowska, Oliver Plümper, Ola Nilsen, and Joanna Dziadkowiec

Interactions between minerals and reactive fluids in porous rocks and building materials often result in crystallization of new minerals. The forces exerted by minerals growing under confinement on the surrounding matrix can be large enough to cause fracturing. Fractures expose new reactive surfaces, leading to progressive disintegration of the material. These processes can result in severe damage to cultural heritage and modern infrastructure, as well as changes in the rheological properties and weathering of natural rocks. Understanding and controlling volume-expanding mineral replacement reactions in pore spaces is thus an important objective to address both societal and geological issues. While crystallization pressures have been measured at larger scales, nanoscale force evolution during confined mineral growth remains poorly constrained.

Here, we investigate volume-expansive mineral reactions in pores spaces by studying the hydration of MgO (periclase) in the Surface Forces Apparatus (SFA). Hydration of MgO to Mg(OH)­2 (brucite) causes a volume increase to 220%, yielding high crystallization pressures. We use MgO thin films (~90 nm) prepared by atomic layer deposition as reactive surfaces in our experiments, which are performed at the Flow Laboratory, Njord Center, University of Oslo. With the SFA, we measure distance-resolved adhesive and repulsive forces acting between two MgO surfaces under variable external load and how these change over time as the reaction progresses. Preliminary results indicate evolution of forces from strongly adhesive to repulsive during the hydration reaction, likely due to the presence of amorphous, gel-like precursors in the early stages of the reaction. As a reference for the SFA experiments, we study the hydration of isolated MgO surfaces with Atomic Force Microscopy (AFM). This allows us to compare nucleation and growth rates, as well as microstructure and porosity of Mg(OH)­2 grown in SFA and AFM.

How to cite: Trautner, V., Rogowska, M., Plümper, O., Nilsen, O., and Dziadkowiec, J.: How hard do crystals push when growing under confinement? Real-time measurements of surface forces during hydration of periclase to brucite, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7493, https://doi.org/10.5194/egusphere-egu26-7493, 2026.

We investigate infiltration of an aqueous fluid into granitic rocks by means of numerical models at the field scale. Our methodology is based on a finite difference approach for solving the transport problem in combination with lookup tables generated from precomputed thermodynamic equilibria covering the compositional space. We also compare results to an approach involving on-the-fly calculation of local equilibrium between fluid and rock. Porosity and density evolution is predicted based on mass conservation. The ability to predict porosity evolution is valuable to better understand applications such as enhanced geothermal systems (EGS). The prediction of reaction zone sequences is also helpful in the understanding of ore deposit formation. We demonstrate how sensitive the metasomatic zoning sequences are to varying rock and fluid composition. As an example, we model metasomatic zone sequences observed in topaz-greisen to show how metasomatic sequences comprising multiple lithologies can be formed in one event with constant incoming fluid composition as boundary condition. Lithological zones formed along fractures do not necessarily imply temporal changes in the fluid composition of the source.

How to cite: Vrijmoed, J. C. and John, T.: Numerical modelling of an aqueous F-Cl-Na-K-Al bearing fluid in local equilibrium with granitic rocks with relevance to enhanced geothermal systems and ore deposit formation., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7508, https://doi.org/10.5194/egusphere-egu26-7508, 2026.

Bedding-parallel fibrous calcite veins in organic-rich shale are commonly regarded as petrographic archives of abnormal pore-fluid overpressure and associated hydrocarbon expulsion and migration. Their formation reflects a dynamic cycle of fracture opening, fluid ingress and mineral precipitation, and subsequent re-opening. Constraining the evolutionary model of BPFVs and evaluating their influence on hydrocarbon accumulation are therefore of clear significance. In lacustrine shale systems, the sources of vein-forming fluids and the extent to which BPFV development couples with organic-matter maturation, overpressure generation, and hydrocarbon accumulation remain poorly constrained. This study investigates lacustrine shale of the second member of the Paleogene Funing Formation (E1f2) in the Qintong Sag, Subei Basin. Core observations, petrographic thin sections, and cathodoluminescence (CL) imaging were used to characterize vein petrography and constrain vein growth stages. Fluid inclusion petrography and microthermometry were conducted to define inclusion assemblages and homogenization-temperature (Th). Carbon–oxygen–strontium (C–O–Sr) isotopes and PAAS-normalized rare earth element (REE) patterns were integrated to diagnose vein forming fluid sources. These datasets were further evaluated against BasinMod-1D burial–thermal–hydrocarbon generation modeling to link Th stages with source-rock maturity and to assess the coupling between BPFVs and hydrocarbon accumulation. The results show that the BPFVs contain a well-defined median zone and symmetric antitaxial fibrous fabrics. Multiple internal growth records indicate repeated fracture opening and sealing. Oil inclusions commonly associated with aqueous inclusions, suggesting that hydrocarbons and formation water entered the bedding-parallel fractures during opening and were co-trapped during vein precipitation. Aqueous-inclusion Th values cluster into two populations (90–100°C and 120–130°C), matching the initial oil window and the main oil generation stage inferred from burial–thermal–hydrocarbon generation histories, and implying at least two vein filling episodes synchronous with source-rock thermal evolution. Geochemical data further show that vein calcite and host-rock carbonates share similar carbon sources and PAAS-normalized REE patterns, with no evidence for high temperature hydrothermal input. These observations indicate that vein forming fluids were dominated by basin-internal diagenetic pore waters, modified by fluids released during hydrocarbon generation and by sustained water–rock interaction. Based on these evidences, we propose a conceptual model for the development of BPFVs. Organic-matter thermal evolution elevates pore-fluid pressure and drives episodic opening of fractures along mechanically weak bedding planes. During opening, these fractures act as short-range pathways for hydrocarbon migration within the shale. Subsequent calcite precipitation partially to completely seals the fractures, preserving time-transgressive fluid properties and migration episodes in veins and fluid-inclusion assemblages. This framework provides key evidence for the dynamic coupling between the formation–evolution of bedding-parallel fractures and hydrocarbon accumulation in lacustrine shale, and offers a reference for reconstructing charging histories and timing in analogous lacustrine shale systems.

How to cite: Cao, S., Zeng, L., and Liu, G.: Fluid Sources of Bedding-Parallel Fibrous Veins in Lacustrine Shales and Their Implications for Hydrocarbon Accumulation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7664, https://doi.org/10.5194/egusphere-egu26-7664, 2026.

EGU26-8135 | ECS | Posters on site | TS1.5

Controls of fault mechanics on mineral precipitation in gold-bearing fault-veins, Indiana Deposit, Northern Chile 

Ashley Stanton-Yonge, Michele Fondriest, Pamela Pérez-Flores, Martin Marquardt, Felipe Reinoso, and José Cembrano

Many epithermal ore deposits form in fault-veins that channel large volumes of vertical fluid flow synkinematic with fault slip. A key genetic process is the interplay among fluid flow, fault activation, and mineral precipitation; however, significant questions remain regarding the mechanics of fault slip under high fluid-flux conditions and its impact on mineralisation. A fundamental question is whether ore deposition is coseismic, post-seismic, or interseismic—specifically, whether pressure drops during seismic rupture are the dominant trigger for mineral precipitation, or whether mineralisation occurs during longer-lived, aseismic creep and sealing cycles. A deeper understanding of these processes is essential for predicting ore grade and spatial distribution.

The Cretaceous Indiana deposit, located in the Coastal Cordillera of northern Chile, is a Cu–Au (Mo–Co) fault-vein system composed of several subvertical NW- or ENE-striking fault veins, with lengths ranging from 300 m to 2 km. Artisanal tunnels provide access to multiple structural levels in oxides and sulphides mineralization, offering exceptional three-dimensional exposure. NW-striking fault-veins host Au–Cu-Fe–Co-rich mineral assemblages associated with pyrite, chalcopyrite, magnetite, actinolite, albite, garnet, epidote, quartz, tourmaline, and late jarosite, clay and hematite. These are cross-cut by ENE-striking fault-veins containing Au–Cu–Mo-Co mineralisation in pyrite and chalcopyrite paragenetically associated with garnet, epidote, actinolite, quartz, and less sericite. High-grade ore shoots commonly occur in dilatational jogs and at the intersections between these two structural sets.

Fault-veins are 1–3 m wide and display complex internal structures. Fault zones of variable thickness occur along the vein margins and mainly record strike-slip motion, expressed as thin (<10 cm) clay-rich gouge bands or thicker (20–80 cm) foliated cataclasites. Ore-bearing veins commonly occur adjacent to these zones and display varied widths, textures, and mineral assemblages. Gold is hosted by quartz or amorphous silica, either free or in pyrite. Brecciated and banded veins record multiple mineralisation events, whereas comb quartz textures with 2–5 cm euhedral crystals indicate slow growth in open space.

Microstructural analyses document multiple episodes of quartz deposition in the form of subparallel and superposed veins that cross-cut clasts of the andesitic host rock. Some brecciated bands contain spherical clasts completely surrounded by concentric cement bands, forming cockade-like structures that suggest fluidised conditions in which cement precipitation occurred while clasts were suspended.

This preliminary evidence indicates the coexistence of long-lived mineralisation processes and cyclic, short-lived deposition events, likely linked to repeated fault activation. Ongoing analyses integrating microstructural observations with mineral chemistry aim to constrain the fault-slip mechanisms responsible for specific mineralisation styles.

How to cite: Stanton-Yonge, A., Fondriest, M., Pérez-Flores, P., Marquardt, M., Reinoso, F., and Cembrano, J.: Controls of fault mechanics on mineral precipitation in gold-bearing fault-veins, Indiana Deposit, Northern Chile, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8135, https://doi.org/10.5194/egusphere-egu26-8135, 2026.

EGU26-8177 | ECS | Orals | TS1.5

Grain-scale residual stress distribution associated with fluid-induced plagioclase breakdown  

Sascha Zertani, Hugo W. van Schrojenstein Lantman, Lisa Kaatz, Alireza Chogani, Oliver Plümper, Luca Menegon, and Timm John

The magnitude and distribution of stress in Earth’s crust is difficult to quantify, but impacts deformation behavior, phase stability, and metamorphic reactions. Stress is influenced by a variety of factors including compositional heterogeneities, volume changes during ongoing reactions, and the influence of far-field stresses. During metamorphic reactions the stress distribution may be modified, but prevailing stresses may also impact reaction kinetics, or which reactions take place. We studied one of the most impactful reactions within the continental crust; the fluid-induced breakdown of plagioclase at high-pressure conditions. The samples are from former lower-crustal granulites exposed on Holsnøy, western Norway. They preserve a reaction front along which the dry granulite is transformed into an eclogite. Reaction progress is intimately linked to fluid ingress and there is no microstructural evidence of deformation. This lack of deformation indicates that the studied microstructures are entirely related to fluid-induced metamorphic reactions. We measured the residual stress associated with plagioclase breakdown by high-angular resolution electron backscatter diffraction and contrasted the results with compositional variations (scanning electron microscope and electron probe micro analyzer). (Scanning) transmission electron microscopy was conducted on selected sites to link this information with the associated dislocation configuration. We find that intragrain residual stress associated with the breakdown of plagioclase is on the order of hundreds of megapascals, and dominantly caused by the elastic interactions of dislocations. Before the reaction plagioclase contains few, randomly oriented dislocations. Compositional modification of plagioclase during the reaction (increasing albite content) leads to dislocations occurring more frequently in the more albitic part of the plagioclase. In that case, dislocations have a preferred orientation, but no significant long-range increase in dislocation density, i.e., increased organization. Our results thus suggest that as plagioclase breaks down, dislocations are mobilized to accommodate the variations in lattice parameters associated with hundreds-of-megapascal stress variations on the grain scale.

How to cite: Zertani, S., van Schrojenstein Lantman, H. W., Kaatz, L., Chogani, A., Plümper, O., Menegon, L., and John, T.: Grain-scale residual stress distribution associated with fluid-induced plagioclase breakdown , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8177, https://doi.org/10.5194/egusphere-egu26-8177, 2026.

EGU26-9041 | Orals | TS1.5

High-pressure metamorphism induced porosity in mafic rocks – wet vs. dry 

Anna Rogowitz, Gerald Degenhart, Jürgen Konzett, Benjamin Huet, Wolfgang Stoiber, and Peter Tropper

Fluid–rock interaction, and thus fluid flow plays a fundamental role in geological processes from the shallow crust to mantle depths. In the upper crust, fluid flow is predominantly controlled by brittle features and interconnected porosity. In contrast, at lower crustal conditions, elevated lithostatic pressures are commonly assumed to inhibit fracturing and major porosity, leaving unresolved how fluids migrate at depth. To investigate porosity development during high-pressure metamorphism of initially impermeable mafic rocks, we conducted a series of piston-cylinder experiments that varied reaction duration and fluid availability. Dolerite from the Kerforne dyke (Brittany, France) was used as starting material. Cylindrical samples (2.8 mm diameter, ~3.5 mm length) were characterized prior to experimentation using X-ray micro-computed microtomography (µCT; 3 µm Isovoxel), enabling three-dimensional quantification of mineral fabric, modal proportions, and initial porosity. The starting dolerite consists of ~50–65% plagioclase, 20–30% pyroxene, up to 10% ilmenite, and minor quartz, with an initial porosity of ~0.1%. The fabric is near-isotropic and dominated by randomly oriented plagioclase grains up to 300 µm in length.

Experiments were performed under quasi hydrostatic conditions at 700 °C and 2.4 GPa for varying durations. To evaluate the influence of fluid availability on reaction progress and porosity evolution, three experimental setups were employed: (1) nominally dry conditions without added fluid, (2) addition of paragonite as a source of fluid and sodium, and (3) addition of 5 vol% water (“wet” conditions). Wet experiments were conducted for durations of 1, 7, and 21 days to assess the temporal evolution of reactions.

Following experimentation, all samples were re-imaged using µCT, allowing three-dimensional mapping of reaction progress and porosity development. Largely unreactive Fe–Ti oxides served as internal markers, enabling accurate registration of pre- and post-experimental µCT datasets and direct comparison between the protolith and reaction products. Three-dimensional observations were complemented by high-resolution two-dimensional analyses using electron probe microanalysis and scanning electron microscopy.
Reaction progress increases systematically with fluid availability, from dry to paragonite-bearing to water-added conditions. Under nominally dry conditions, reactions are restricted to narrow zones along pyroxene–plagioclase interfaces and plagioclase grain boundaries, producing predominantly fine-grained zoisite needles (<5 µm). In paragonite-bearing experiments, reaction intensity increases within plagioclase, characterized by the growth of zoisite and phengite, while jadeite forms along pyroxene–plagioclase boundaries. In contrast, wet experiments result in complete replacement of plagioclase within 7 days by an assemblage of zoisite, phengite, amphibole, and minor omphacite and quartz. Pyroxene develops narrow reaction rims (<30 µm wide) marked by increasing Al and Na and decreasing Fe and Ca contents, while garnet occurs as idiomorphic grains in the fine-grained matrix or as coronae surrounding oxides.
Porosity development is closely coupled to reaction progress, and three distinct porosity types are identified: (1) micro- to nanopores within plagioclase reaction products, (2) nanopores within pyroxene reaction rims, and (3) microfractures. The first two porosity types are interpreted to result from volume reduction associated with density increases during metamorphic reactions, whereas microfractures likely form in response to stress concentrations and elevated pore-fluid pressures.  

How to cite: Rogowitz, A., Degenhart, G., Konzett, J., Huet, B., Stoiber, W., and Tropper, P.: High-pressure metamorphism induced porosity in mafic rocks – wet vs. dry, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9041, https://doi.org/10.5194/egusphere-egu26-9041, 2026.

The presence or absence of fluids strongly affects rock rheology. Lawsonite is a very hydrous mineral (~12 wt.% H2O), characteristic of cold subduction zones. Its destabilization may generate fluid overpressure, reduce effective stress, and trigger brittle failure through dehydration embrittlement. On the other hand, its H2O-consuming growth may deplete available fluids from the matrix and drive the rock dry. The quantity of lawsonite, the locus of maximum dehydration, and the amount of fluids produced/consumed depend on the pressure-temperature (P-T) path of the subducted crust. An accurate interpretation of P-T paths of natural blueschists is therefore crucial.

At Ile de Groix (Armorican Massif, France), garnet-bearing blueschists display cm-sized lawsonite pseudomorphs smoothly wrapped by an epidote- and glaucophane-bearing foliated matrix. Both garnet and pseudomorphed lawsonite porphyroblasts contain sigmoidal inclusion trails of fine-grained oriented epidote, glaucophane and titanite, continuous with the matrix schistosity. Garnet is zoned (rimward decrease of Mn and increase of Mg) and locally included in pseudomorphed lawsonite. Lawsonite pseudomorphs comprise coarse unoriented epidote, paragonite and chlorite. Textural analysis therefore suggests a prograde synkinematic growth of garnet and lawsonite in an epidote-bearing matrix. In the light of calculated phase diagrams, this points to a prograde P-T path dominated by a near-isothermal compression from LT epidote-blueschist facies toward peak pressure conditions in the epidote + lawsonite stability field, at ~19 kbar and ~550°C, consistent with garnet rim composition and modal proportions of major phases. 

Thermodynamic modeling further indicates that lawsonite growth in an epidote-bearing blueschist leads to the complete consumption of free fluid, resulting in a dry, fluid-absent rock near peak pressure conditions. However, dry rocks are commonly stronger than their wet equivalents. Our results thus suggest that, contrary to common expectations, hydration reactions may locally induce an increase in rock strength, as exemplified by lawsonite crystallization during the prograde transition from epidote- to lawsonite-blueschist subfacies. Such reactions could provide an explanation for earthquakes occurring within the lawsonite stability field, well prior to its destabilization.

How to cite: Pichouron, R., Pitra, P., and Yamato, P.: Prograde P-T path of lawsonite-bearing blueschists: insights from Ile de Groix and implications for fluid content and rheology of subducted oceanic crust, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9564, https://doi.org/10.5194/egusphere-egu26-9564, 2026.

EGU26-10026 | ECS | Orals | TS1.5

Experimental constraints on the kinetics of the albite = jadeite + quartz reaction depending on grain size and reaction overstepping 

Simon Schorn, Zongpeng Yang, Friedrich Hawemann, Stephan Buhre, Roman Botcharnikov, and Evangelos Moulas

Densification and deformation during eclogitization govern the strength and buoyancy of orogenic roots and the stability of mountain ranges over geological timespans. The breakdown of albite to jadeite + quartz represents a key end-member reaction that is associated with densification of about 20%; shear stresses induced by such volumetric changes may cause brittle failure and have been linked to intermediate-depth seismicity (Yamato et al., 2022). Eclogitization is a kinetically sluggish process that requires significant reaction overstepping and may proceed far beyond the equilibrium pressure–temperature conditions, and/or remain largely incomplete – particularly in fluid-deficient felsic crust as evidenced by field observations (Palin et al., 2017) and geophysical constraints (Hetényi et al., 2021). However, the kinetics of the albite = jadeite + quartz reaction is poorly constrained, especially regarding the roles of grain size, pressure–temperature overstepping, and reaction duration. To address this gap, we conducted high-pressure experiments using a piston-cylinder apparatus at the Institute of Geosciences, JGU Mainz. Natural albite crystals were crushed and sieved into grain size fractions between 50 and 500 µm, loaded into Au-capsules, and separated by Au-foils. A subset of experiments involved furnace-drying (~500°C) of the starting materials followed by hot-welding of the capsules to minimize atmospheric moisture contamination. In experimental stage I, pressure was initially set just below (~1 kbar) the albite = jadeite + quartz reaction boundary (Holland, 1980), followed by heating to target temperature. In stage II, pressure was increased at constant temperature to variable target pressures above the reaction to systematically explore the effect of reaction overstepping. Samples where quenched by power shutdown, and reaction progress was quantified using scanning electron microscopy (backscattered electron imaging and cathodoluminescence) based on the relative fractions of reactant albite and products jadeite–quartz. Preliminary results reveal highly variable degrees of reaction progress. Where present, jadeite–quartz occur as finely intergrown symplectites, typically decorating albite grains at the rims, as well as forming within larger albite grains. The latter textures indicate complications arising from fluid inclusions in the starting material. By combining constraints on P(T) overstep, grain size, and experimental run duration, we determine effective reaction rates for albite breakdown. These results provide end-member kinetic constraints on high-pressure transformation in fluid-deficient, coarse-grained felsic rocks, which constitute the bulk of many well-known (U)HP terranes such as the Western Gneiss Region (Norway) and the Dabie–Sulu belt (China).

References

Hetényi, G. et al. (2021). Metamorphic transformation rate over large spatial and temporal scales constrained by geophysical data and coupled modelling. Journal of Metamorphic Geology, 39(9), 1131–1143.

Holland, T. J. (1980). The reaction albite = jadeite + quartz determined experimentally in the range 600–1200°C. American Mineralogist, 65(1-2), 129–134.

Palin, R. et al. (2017). Subduction metamorphism in the Himalayan ultrahigh-pressure Tso Morari massif: an integrated geodynamic and petrological modelling approach. Earth and Planetary Science Letters, 467, 108–119.

Yamato, P. et al. (2022). Reaction-induced volume change triggers brittle failure at eclogite facies conditions. Earth and Planetary Science Letters, 584, 117520.

How to cite: Schorn, S., Yang, Z., Hawemann, F., Buhre, S., Botcharnikov, R., and Moulas, E.: Experimental constraints on the kinetics of the albite = jadeite + quartz reaction depending on grain size and reaction overstepping, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10026, https://doi.org/10.5194/egusphere-egu26-10026, 2026.

EGU26-10373 | ECS | Orals | TS1.5

Evolving fluid pathways in a shallow mega-thrust shear zone (Northern Apennines, Italy) 

Martina Rocca, Silvia Mittempergher, Francesca Remitti, Giancarlo Molli, Marta Gasparrini, Friedrich Hawemann, Renato Diamanti, Nereo Preto, and Telemaco Tesei

Megathrust shear zones are weak interplate faults that accommodate deformation under low effective stress in a fluid-rich environment. The evolution of stress and fluids during megathrusts activity can be reconstructed from syn- and post-tectonic mineral veins in exhumed settings.

The Sestola–Vidiciatico Unit (SVU) in the Northern Apennines is a fossil analogue of a shallow subduction megathrust mélange. It represents the plate boundary shear zone (200–400 m thick) between the Ligurian prism and the underthrusted Adria microplate active during the early–middle Miocene with peak temperatures of ~170 °C. The SVU is composed of kilometre-scale slices of marls, shales and sandstones derived from the Ligurian prism and its sedimentary cover, thrust along a basal décollement onto younger Adria-derived foredeep turbidites.

This study focuses on a well-exposed outcrop along a south-dipping thrust ramp of the basal décollement of the SVU. The footwall consists of sandstones and siltstones of Langhian age, overthrust by a slice of Aquitanian marls, and by an upper slice of Priabonian – Bartonian claystone. We performed structural mapping, microstructural and geochemical analyses (O-C stable isotopes, trace and major element geochemistry), and fluid inclusion studies on calcites filling shear and extensional veins and cementing tectonic breccias.

Marls and claystones within the SVU are bounded by sharp thrust surfaces decorated by multiple generations of shear veins. In the vicinity of the main thrusts, marls and claystone are crosscut by pervasive shear fractures, bounding flattened and elongated lithons defining a foliation at low angle to the thrusts. Deformation in the footwall includes oblique cleavage, bedding-parallel shear planes, and a conjugated set of NNE-SSW left-lateral and N-S trending right-lateral subvertical transtensional faults showing mutually crosscutting relationships with the basal thrust of the SVU. Calcite shear veins mark thrust surfaces, whereas transtensional faults in the footwall are marked by shear and extension veins, as well as calcite-cemented breccias. Two different calcite phases have been observed: an early-stage calcite, rich in host-rock inclusions and a later inclusion-free calcite.

Geochemical and thermometric results point to two groups of distinct mineralizing fluids circulating through the fracture network: (1) diluted seawater precipitating early-stage calcites at low temperatures (< 50 °C up to 70 °C); (2) an external low-salinity fluid precipitating later-stage calcites at higher temperatures (~80-100° C).

Our data suggest a transition from low temperature and low salinity fluids, possibly from mixing of seawater and fluids released from clay dehydration during progressive burial of the SVU, to the ingression of moderately hot fluids (up to 120 °C) external from the system. This indicates that the onset of fluid circulation by faulting is modulated by the embrittlement and seismic ruptures in subduction zones, favoured by a low-stressed environment.

How to cite: Rocca, M., Mittempergher, S., Remitti, F., Molli, G., Gasparrini, M., Hawemann, F., Diamanti, R., Preto, N., and Tesei, T.: Evolving fluid pathways in a shallow mega-thrust shear zone (Northern Apennines, Italy), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10373, https://doi.org/10.5194/egusphere-egu26-10373, 2026.

EGU26-11740 | ECS | Posters on site | TS1.5

Carbonate concretions as proxy for methane-enriched fluid flow in high-porosity sandstone: example from Crotone forearc Basin, Italy 

Mattia Pizzati, Luigi Riccardo Berio, Cristian Cavozzi, Anita Torabi, and Fabrizio Balsamo

Diagenetic processes exert a strong control on reservoir potential, heavily impacting the exploitation of strategic fossil resources (oil and gas), preservation and management of aquifers, and underground storage of anthropogenic CO2. Therefore, in high porosity media such as sandstones, the study of selective cementation is crucial to the quantification of reservoir properties and quality. The outcrop-based analysis of cementation types and patterns could unravel fossil fluid flow pathways affecting porous reservoir analogues.

This study is focused on the selective cementation of fluvio-deltaic, Lower to Middle Pliocene age, sandstone to conglomeratic bodies exposed in the Crotone forearc Basin, South Italy. The siliciclastic unit was deposited in a shallow marine setting and reaches a maximum thickness of ~200 m, unconformably overlying the Paleozoic Sila Massif metamorphic basement. The sandstone sequence is almost devoid of diagenetic cement thus preserving most of the original primary porosity. Sandstone beds show a gentle tilting towards SE, with mild brittle deformation in the form of deformation bands and low-displacement faults. Selective cementation of host sandstone can be traced as diagenetic concretions of different shapes and sizes. Concretion types span from tabular-lens shaped with lateral extension up to 10’s m, elongate blade-shaped from 10 cm up to several 10’s meter-long, asymmetric drop-shaped and nodular-spherical bodies. The elongation direction of concretions parallels the southeastward dip of bedding surfaces, while in the vicinity of deformation bands and faults, elongate concretions are parallel to their dip. Pervasive calcite precipitation was responsible for the dramatic porosity loss from 27-32% down to 2-3%, leading to an increase in sandstone cohesion and stiffness. The stiffness increase can be documented in tightly cemented bodies that host 2-3 sets of joints abutting at the concretion-host rock boundary. Cold cathodoluminescence revealed the ubiquitous presence of bright yellow, granular to poikilitic calcite cement in all concretions. Carbon and Oxygen stable isotopes of calcite cement suggest two fluid sources responsible for the selective cementation. The first source can be traced in weakly cemented lens-shaped bodies and along secondary faults and is made of mixed marine-meteoric fluids with contributions from soil percolation. Conversely, the second source can be detected in tightly cemented lens-shaped and nodular to elongate concretions and is given by a mix of marine fluids with contributions from biogenic methane likely related to biological-bacterial activity in a shallow marine setting. The evolution of fluids from meteoric to marine can be associated with a transgressive sea level rise and upward basin-boundary fault propagation that occurred during and after sandstone deposition. The source of methane could be traced in the thick evaporitic (gypsum and anhydrite) sequence underneath the studied sandstone formation, providing large volume of biogenic methane. Methane enriched fluids migrated vertically following major basin-boundary faults permeating the high porosity sandstone and mixed with meteoric to marine fluids providing bed-parallel fluid flow imparted by the hydraulic and topographic gradient.

How to cite: Pizzati, M., Berio, L. R., Cavozzi, C., Torabi, A., and Balsamo, F.: Carbonate concretions as proxy for methane-enriched fluid flow in high-porosity sandstone: example from Crotone forearc Basin, Italy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11740, https://doi.org/10.5194/egusphere-egu26-11740, 2026.

EGU26-12642 | ECS | Posters on site | TS1.5

Grain boundary processes from the deep continental crust to the surface (ICDP-DIVE, Drilling the Ivrea-Verbano Zone) 

Etienne Linden, Friedrich Hawemann, Marco Venier, and Virginia Toy and the DIVE science Team

Fluid transport, precipitation and accompanying mineral reactions along grain boundaries are among the most important processes impacting the rheology of the crust and the formation of mineral deposits. Porosity and permeability that constantly evolve during fluid flow govern major petrophysical properties of the rock. Most commonly, rocks are investigated in two-dimensional sections, where grain boundaries appear as thin lines and the three-dimensional structure cannot be captured. Computed tomography allows for a quantitative assessment of pore space but has a limited resolution. Additionally, it is difficult to assess the origin of pores, which may have been formed primarily in the crust or during near surface weathering or sampling.

In this study, we investigated grain boundaries directly using the “broken surface” technique: A cm-sized rock slice was broken and platinum-coated for scanning electron microscopy. In favorable cases, the rock slice broke along grain boundaries and pre-existing small-scale fractures, exposing these structures directly as true surfaces rather than sectioned traces. The samples investigated are from the ICDP-DIVE drilling project in the Ivrea Verbano Zone (Italy), an exhumed section of the lower continental crust, spanning the range of tens of meters to hundreds of meters of depth below surface; thus offer information about which grain boundary decorations can be clearly related to near-surface alteration. In addition, we compare samples from both amphibolite and granulite facies rocks to explore variations between supposedly fluid-rich and fluid-poor conditions.

Our observations contribute to the understanding of grain boundary processes through a catalogue of different features observed and interpreted, including, among other processes: formation of clays near the surface, sulfide precipitation, quartz recrystallisation and sericitization of feldspars.

How to cite: Linden, E., Hawemann, F., Venier, M., and Toy, V. and the DIVE science Team: Grain boundary processes from the deep continental crust to the surface (ICDP-DIVE, Drilling the Ivrea-Verbano Zone), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12642, https://doi.org/10.5194/egusphere-egu26-12642, 2026.

EGU26-12738 | ECS | Orals | TS1.5

Migration pathways of crustal and mantle fluids during the formation of the Betic Cordillera (SE Spain). 

Bérénice Cateland, Anne Battani, Frédéric Mouthereau, Matthias S. Brennwald, Antonio Caracausi, Benjamin Lefeuvre, and Magali Pujol

Crustal-to-lithospheric-scale strike-slip faults can act as major pathways for crustal and mantle fluids, with implications for natural resources (e.g., geothermal, ore deposits) as well as natural gas storage and migration. The Betic Cordillera (SE Spain) records a complex geodynamic evolution, from slab retreat, tearing and delamination to the later inversion of a thinned continental margin. This extreme crustal thinning (~15 km) associated with metamorphic dome exhumation during the Miocene was accommodated by crustal to lithospheric-scale faults that are still active today (e.g. the Mw 5.2 Lorca earthquake in 2011).

To determine the geochemical origin of fluids, their migration pathways, and fault-controlled permeability through time, we analyzed noble gases (He, Ne, Ar) as inert, non-reactive geochemical tracers in both paleo- and present-day fluids. Noble gases in paleo-fluids were analyzed in quartz and calcite minerals associated with faults (INGV, Palermo). We also analyzed noble gases dissolved in water discharged from thermal springs at ~20 to 53°C (Eawag/ETH Zürich).

In calcite and thermal water, low ³He/⁴He ratios (R/Ra ≤ 0.5) indicate mixing between a dominantly crustal component and a mantle contribution or a mixed crustal-atmospheric origins. Quartz samples show stronger atmospheric contamination than in calcite, although ⁴⁰Ar/³⁶Ar ratios may suggest deep input (mantle vs crust; ⁴⁰Ar/³⁶Ar values between 490 and 1215). He-Ne isotopes in paleo-fluids reveal two areas that show a likely mantle-derived noble gas signature: Sierra Elvira, with ~3% mantle contribution suggested, and the Carboneras Fault Zone, with ~6%. In contrast, present-day fluids could reflect a ~4% mantle contribution in the northeastern Betics at Mula and Archena. We infer that mantle-derived signatures detected in paleo-fluids are not preserved in the same locations in present-day fluids. For instance, along a single fault system (e.g., the Carboneras Fault), paleo-fluids display up to four times higher mantle contributions (Rc/Ra ≈ 0.5) than present-day fluids (Rc/Ra ≈ 0.1). This contrast opens new questions regarding potential changes in mantle fluid sources or migration pathways during the evolution of the Betic Cordillera, the impact of tectonic inversion on deep fault permeability, the residence time of fluids in the crust, and the role of fault geometry in controlling fluid pathways.

How to cite: Cateland, B., Battani, A., Mouthereau, F., Brennwald, M. S., Caracausi, A., Lefeuvre, B., and Pujol, M.: Migration pathways of crustal and mantle fluids during the formation of the Betic Cordillera (SE Spain)., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12738, https://doi.org/10.5194/egusphere-egu26-12738, 2026.

In deep sedimentary basins, the formation and evolution of fracture-vein systems are critical for understanding fluid migration and overpressure history. This study investigates antitaxial fibrous illite veins in the Upper Triassic Xujiahe Formation of the Wubaochang area, Sichuan Basin, to decipher the mechanisms of fluid overpressure and diagenetic evolution. A multi-proxy approach was employed, combining detailed petrography, SEM, and micro-XRD. Crucially, we applied Optical Photothermal Infrared Spectroscopy (O-PTIR)  to achieve sub-micron resolution mapping of organic functional groups within single illite fibers, alongside in-situ REE and C-O isotope analysis. Detailed petrography and SEM analysis reveal that these veins exhibit typical antitaxial growth characteristics, where mineral fibers grow from a median plane toward the host rock, recording the continuous opening and synchronous filling of fractures. In-situ rare earth element (REE) and carbon-oxygen (C-O) isotope analyses identify two distinct fluid evolution stages: Stage I reflects an external, deep-circulating basin fluid system driven by regional tectonic stress, characterized by significant water-rock interaction with host rocks. Conversely, Stage II represents localized diagenetic and hydrocarbon-generated fluids, where isotopic signatures shift toward organic-derived carbon sources, indicating a transition to hydrocarbon-generation-induced overpressure. To definitively address the timing of fluid injection, sub-micron resolution O-PTIR (Optical-Photothermal Infrared) analysis was conducted, revealing the simultaneous presence of organic acid (1720cm-1), aromatic (1600cm-1), and aliphatic (1450cm-1) functional groups coexisting with the illite lattice vibration (1034 cm-1) within single fibrous crystals. The high ratio of organic acids to mineral signals indicates that organic acids directly mediated water-rock reactions and mineral precipitation rather than being late-stage infiltrations. Our findings demonstrate that these fibrous veins are coupled products of tectonic-induced fracturing and organic-acid-mediated mineral growth. This study highlights the power of O-PTIR as a novel tracer for deciphering organic-inorganic interplays, offering new insights into the mechanisms of fluid overpressure and hydrocarbon expulsion in deep, complex basin systems.

How to cite: Wang, Z., Zeng, L., and Gasparrini, M.: Fluid overpressure and diagenetic evolution recorded by antitaxial fibrous illite veins in deep coal-bearing strata: Insights from sub-micron O-PTIR and in-situ geochemistry, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14497, https://doi.org/10.5194/egusphere-egu26-14497, 2026.

EGU26-15103 | Orals | TS1.5

Interplay between alteration and damage at the Nojima fault zone (Japan) revealed by borehole geophysics 

Mai-Linh Doan, Maxime Jamet, Romain Iaquinta, Benoît Gibert, Patricia Patrier, and Yann Lucas

Large active faults tend to differ from younger, fresh faults. They are the loci of the greatest earthquakes, but they often creep. The damage zone thickness tends to saturate with large displacement. Deep scientific drilling in large active faults systematically reveals differentiated fault gouge surrounded by a halo of fracturing and alteration. Despite its importance for fault evolution, the process of alteration in large active faults remains poorly understood.

After the devastating Mw 6.9 Nanbu-Kobe earthquake of 1995, a 750 m deep borehole was drilled into the Nojima fault, reaching the fault core at 625 m. The Hirabayashi borehole was drilled ~1 year after the earthquake and provided an extensive dataset on the structure of the fault where the earthquake originated. Continuous coring and borehole geophysics conducted within the borehole showed that the granodiorite protolith experienced several stages of alteration, including fault-related alteration that produced for example laumontite (Ca-rich zeolite) and smectite at T>150°C.

The ANR project AlterAction is revisiting this data with a multidisciplinary team to better understand the interplay between alteration and fault deformation, with 3D imaging of the core samples (see presentations by Romain Iaquinta and Maxime Jamet) and systematic petrophysical characterization.

This presentation will focus on the reanalysis of geophysical logs. Sonic velocities, electrical resistivities, and lithodensities progressively decrease when approaching the fault, starting to deviate from the protolith rock. In the granitoid rocks composing the borehole, variations in gamma-ray may reflect changes in the protolith rather than alteration. This fault zone starts at 370 m (255 m above the fault core) in the hanging wall, with a more pronounced decrease below 540m (85 m above the fault core, corresponding to a zone of thickness ~8 m, given the well trajectory, which is almost tangent to the fault dip). In the footwall, the strong decrease extends down to 680 m (55 m long zone), with lower velocities, resistivities and densities between 625 and 635m, below the fault core. Crossplotting the logging dataset shows the same trends, whether in the footwall or the hanging wall, regardless of the distance to the fault. This suggests that most of the fault zone is affected by the same interplay between alteration and damage. The fault core (623-626m) is singular owing to its relatively large sonic velocities, suggesting that sealing was strongly localized and effective in the fault core one year after the earthquake.

How to cite: Doan, M.-L., Jamet, M., Iaquinta, R., Gibert, B., Patrier, P., and Lucas, Y.: Interplay between alteration and damage at the Nojima fault zone (Japan) revealed by borehole geophysics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15103, https://doi.org/10.5194/egusphere-egu26-15103, 2026.

EGU26-15694 | ECS | Posters on site | TS1.5

Reaction-induced fracturing and rheological effects of carbonation at the slab–mantle interface: Constraints from hydrostatic and shear experiments 

Shunya Okino, Atsushi Okamoto, Ryosuke Oyanagi, Yukiko Kita, Sando Sawa, and Jun Muto

Ultramafic rocks are increasingly recognized as promising reservoirs for long-term carbon fixation through mineral carbonation. However, carbonation reactions are inherently self-limiting, as they involve solid volume increases of up to ~68%, which clog pore spaces, drastically reduce permeability, and inhibit further fluid infiltration. Geological processes capable of sustaining permeability during carbonation have therefore been invoked, including (1) continuous tectonic deformation that generates microfractures (Menzel et al. 2022, Nat. Commun.), and (2) metasomatic mass transfer from mantle rocks to the crust that reduces net solid volume (Okamoto et al. 2021, Commun. Earth Environ.). Despite their importance for both natural and engineered carbon storage, the dynamic coupling between metasomatic reactions, volumetric changes, and deformation remains poorly constrained by experiments.

Here we investigate reaction–deformation coupling at the slab–mantle interface using a series of hydrostatic and shear deformation experiments conducted at 500 °C and 1.0 GPa in a Griggs-type piston-cylinder apparatus. Experimental assemblies consisted of a three-layer configuration in which a crustal lithology (pelitic schist from the Sanbagawa belt or quartzite) was sandwiched between harzburgite (Horoman peridotite) and serpentinite (Mikabu belt). Hydrostatic experiments were performed with pure H₂O, whereas shear experiments employed H₂O–CO₂ fluids (XCO₂ = 0.2) generated in situ by thermal decomposition of oxalic acid dihydrate.

Hydrostatic experiments reveal that metasomatic reaction pathways and resulting textures are strongly controlled by the chemical composition of the adjacent crustal rock. In experiments involving pelitic schist, albite phenocrysts are preferentially replaced by Mg-rich saponite, while talc precipitates within dendritic fracture networks in the serpentinite. Mass balance calculations indicate that Mg absorption by Al-bearing minerals in the sedimentary rocks promotes progressive Mg extraction from mantle lithologies. Importantly, textural contrasts between lithologies indicate opposite volumetric responses: reaction-induced fracturing in serpentinite is associated with net solid volume reduction, whereas reactions in harzburgite proceed with solid volume expansion.

Shear deformation experiments conducted along quartzite–serpentinite interfaces exhibit a pronounced reaction-duration dependence on mechanical behavior. Short time reaction (6 h), friction coefficients are relatively high. In contrast, long reaction duration (68 h) results in stable sliding with exceptionally low friction coefficients. Microstructural observations show the development of a reaction zone dominated by extensive carbonation (listvenite formation: quartz + magnesite) localized at the lithological interface. Deformation is strongly localized within the carbonation products, which display laminar fabrics and magnesite-filled fractures containing nanoscale porosity.

Integrating hydrostatic and shear experiments, we suggest that metasomatic mass transfer is essential for sustaining carbonation reactions. Furthermore, the pronounced mechanical weakening observed in shear experiments may not be solely attributable to talc precipitation, but possibly also to the dehydration accompanying carbonation. Instead, the dynamic coupling between chemical reactions, solid volume changes, and deformation promotes fracture formation, permeability maintenance, and extreme rheological weakening. These processes provide a viable mechanism for overcoming reaction-induced pore clogging during long-term carbonation and have profound implications for carbon transport, storage efficiency, and the mechanical behavior of the slab–mantle interface.

How to cite: Okino, S., Okamoto, A., Oyanagi, R., Kita, Y., Sawa, S., and Muto, J.: Reaction-induced fracturing and rheological effects of carbonation at the slab–mantle interface: Constraints from hydrostatic and shear experiments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15694, https://doi.org/10.5194/egusphere-egu26-15694, 2026.

EGU26-15970 | Orals | TS1.5

Linking Reactive Fluid Flow to Rheology of Eclogite-Facies Oceanic Crust 

Andrew Smye, Leonie Strobl, Hailey Forgeng, and Don Fisher

During subduction, progressive heating and burial drive dehydration reactions that release H₂O-rich fluids from altered oceanic crust. Under sub-arc conditions (2–4 GPa), the transition from blueschist- to eclogite-facies mineral assemblages is accompanied by the release of substantial amounts of water (up to ~5 wt.%). If fluid transport occurs on timescales that are short relative to subduction, these fluids migrate through the overlying oceanic crust into the mantle wedge or along the slab–wedge interface. This process is critical for the generation of arc magmas and for their enrichment in fluid-mobile trace elements. Despite the importance of this process, relatively few direct constraints exist on the extent to which such fluids react with the eclogite-facies crust through which they migrate.

Here, we present field, petrological and geochemical observations from a pristine suite of transport veins preserved in mafic eclogites of the Tauern Window, Eastern Alps. The veins are dominated by high-variance, quartz-rich mineral assemblages and are surrounded by well-developed, omphacite-dominated selvages. Phase equilibrium modeling indicates that vein formation occurred at or near peak pressure–temperature conditions of ~2.5 GPa and ~600 °C. A striking feature of the fluid–rock interaction is the near-complete consumption of garnet by the reactive fluid. Trace-element zoning in partially reacted garnet porphyroblasts records a fluid-driven dissolution–precipitation mechanism that mobilized middle and heavy rare earth elements (MREE and HREE). Isocon analysis of the altered eclogite selvages reveals bulk gains in Na and Li, accompanied by losses of REE, Sr, K, Cu, Fe, Al, Y, Mn, Ba, and Cr, while Ni, Sc, and Ti appear to have been conserved.

Pure omphacite layers and seams are commonplace throughout the Eclogite Zone and are interpreted as sealed transport veins. The associated microstructures record embrittlement and fracturing following fluid–rock interaction. Collectively, these observations indicate that reactive fluid flow under eclogite-facies conditions may influence the rheology of subducting oceanic crust.

How to cite: Smye, A., Strobl, L., Forgeng, H., and Fisher, D.: Linking Reactive Fluid Flow to Rheology of Eclogite-Facies Oceanic Crust, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15970, https://doi.org/10.5194/egusphere-egu26-15970, 2026.

EGU26-16106 | Posters on site | TS1.5

Triple oxygen isotope evidence for modified seawater during low-temperature submarine silicate alteration and weathering 

Justin Dodd, Gavin Piccione, Daniel Ibarra, David McNamara, Gabriel Pasquet, Melody Lindsay, Deborah Eason, Anne Briais, Ross Parnell-Turner, and Leah LeVay

The extent to which ambient seawater permeates and interacts with submarine lithologies (e.g., sediments and seafloor basalt) is a critical constraint on the timing and rate of in situ subseafloor silicate weathering. Oxygen isotope (δ18O) values of low-temperature silicate minerals in the marine record often present seemingly inconsistent oceanographic and diagenetic histories. These uncertainties largely arise because neither formation temperature (e.g., burial or alteration) nor the modification of seawater δ18O values through water–rock interactions are well constrained. However, the triple oxygen isotope (Δ17O) approach provides additional constraints on the diagenetic temperature and seawater modification. 

Here we present two case studies of Δ17O variations in low-temperature silicate minerals from widely disparate marine settings that represent potential endmembers in subseafloor diagenetic environments and seawater modification through water–rock interactions. Marine sediment cores from the Ross Sea, Antarctica, collected during IODP Expedition 374 and the ANDRILL McMurdo Ice Shelf program, contain well-preserved biogenic opal (diatomite) of Pleistocene to middle Miocene age (~2.2–16.5 Ma). The mineral structure of opal from these sites (IODP U1521 and U1523; AND-1b and AND-2a) ranges from opal-A to chert, and the Δ17O values reflect isotopic equilibrium with a significantly modified seawater at a range of temperatures consistent with the geothermal gradient and burial depth. Measured Δ17O values for all opal samples fall below the seawater equilibrium curve and likely reflect equilibration with pore waters. The abundance of hydrous mineral phases (e.g., mirabilite, authigenic clays) in the Ross Sea cores suggest that water-rock interactions may have altered the pore water Δ17O values. Pore water δ18O values and chemistry at the ANDRILL sites suggest the presence of a cryogenic brine with a low δ18O value; however, in the IODP sites on the continental shelf and slope, pore water δ18O values are closer to that of modern Ross Sea Bottom Water. In a very different geologic setting in the North Atlantic, similarly modified seawater Δ17O values are recorded in alteration minerals (e.g., celadonite, saponite, and zeolite) in submarine basalt veins/vesicles from IODP Site U1564, which is located east of the Reykjanes Ridge in ~32.4 Ma crust. The alteration minerals Δ17O values appear to show a mixing relationship between seawater and unaltered basalt endmember with varying water–rock ratios and/or formation temperatures, which suggests fluid evolution or mixing of fluids with different Δ17O values. Observed Δ17O values in ancient geologic materials (e.g. Archean cherts) have been interpreted as reflecting primary oceanographic conditions or subsequent diagenetic alteration by meteoric waters. In the geologic settings described here, the Δ17O variability appears to record significant in situ subseafloor modification of seawater oxygen isotope values through low-temperature water–rock interactions. Constraining the timing and extent of water–rock interactions are, therefore, essential for refining models of geochemical reactions, fluid flow, global element cycling, and deep-biosphere microbial processes in the marine subseafloor environment.

How to cite: Dodd, J., Piccione, G., Ibarra, D., McNamara, D., Pasquet, G., Lindsay, M., Eason, D., Briais, A., Parnell-Turner, R., and LeVay, L.: Triple oxygen isotope evidence for modified seawater during low-temperature submarine silicate alteration and weathering, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16106, https://doi.org/10.5194/egusphere-egu26-16106, 2026.

EGU26-16117 | ECS | Orals | TS1.5

Monazite occurrence and low-temperature alteration in river sediments from contrasting tectonostratigraphic units in southwestern Taiwan 

Han Lin Yeh, Yu Ting Wang, Chien Che Huang, and Yen Hua Chen

Monazite from placer deposits along the southwestern coast of Taiwan was previously exploited as a source of rare earth elements (REEs). However, the formation mechanisms of the distinct monazite types remain debated and are commonly attributed to fluid-related processes. Due to the extremely high denudation rates of rivers in Taiwan, sediments undergo rapid transport, allowing the protolith characteristics of their provenance to be preserved. In this study, we examine river sediments from the Zengwen, Ailiao, and Laonong Rivers, which drain contrasting tectonostratigraphic units within each catchment. We characterize the occurrence and elemental distributions (e.g., La, Th, Nd) of monazite and examine the REE geochemical behavior of the bulk sediments. This study provides a comprehensive mineralogical and geochemical assessment of monazite associated with specific tectonostratigraphic units, offering constraints on sediment provenance.

Preliminary results summarize the variations in monazite occurrence and alteration across different tectonostratigraphic units. In the sediments of the Zengwen River, which primarily drains the Western Foothills, we observed a predominance of detrital monazite (<10 µm), as well as monazite associated with TiO2, apatite, and clay minerals. These features suggest an origin primarily from the physical weathering of detritus or minor fluid precipitation, differing significantly from the occurrences of monazite found on the southwest coast.

Sediments from the Ailiao and Laonong rivers, which drain low-grade metamorphic rocks of the Central Range, exhibit evidence for variable degrees of low-temperature alteration affecting primary monazite. This includes inclusion-hosted, morphologically black monazite comparable to that observed along the southwestern coast of Taiwan. In the Laonong River, which additionally drains the Western Foothills, monazite occurs either within quartz grains or within the interlayers of clay minerals, similar to that observed in the Zengwen River. Furthermore, in rivers originating from the Slate Belt, in addition to monazite as a heavy mineral, we identified pyrite spherules comparable to those in the slate host rocks, as well as xenotime associated with thorite. Overall, these observations reveal distinct patterns in monazite occurrence and alteration among different tectonostratigraphic settings, with implications for sediment provenance in high-denudation river systems.

How to cite: Yeh, H. L., Wang, Y. T., Huang, C. C., and Chen, Y. H.: Monazite occurrence and low-temperature alteration in river sediments from contrasting tectonostratigraphic units in southwestern Taiwan, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16117, https://doi.org/10.5194/egusphere-egu26-16117, 2026.

EGU26-16249 | ECS | Posters on site | TS1.5

Classification and Provenance of Monazite in the Zhuoshui River System, Taiwan 

Po-Cheng Yang and Yan-Hua Chen

Monazite is a phosphate mineral that contains Rare-Earth Elements (REEs), whose micro-textures and chemical compositions can serve as effective indicators of sediment provenance. In Taiwan, monazite in fluvial and coastal sediments may reflect contributions from both external sources and orogenic recycling; however, a systematic classification framework and provenance constraints for monazite in major river systems remain limited. This study focuses on the Zhuoshui River catchment and establishes a monazite classification scheme based on integrated microtextural and geochemical characteristics, which is then applied to assess the provenance of the monazite.

    Bedrock and riverbed sediment samples were collected from the upper reaches and along the Zhuoshui River system during both wet and dry seasons. Scanning Electron Microscope (SEM) backscattered electron (BSE) imaging and semi-quantitative Energy Dispersive Spectrometer (EDS) analyses were used to characterize grain morphology, inclusion features, and REE–Th–Y elemental systematics. The results show that monazite populations and La/Ce systematics are consistent between wet- and dry-season samples, indicating that the provenance signal is stable and not significantly affected by seasonal hydrological variability.

  Based on REE proportions, grain morphology, and inclusion characteristics, monazite grains can be classified into three types. Detrital monazite is generally larger, inclusion-free, relatively enriched in Th, and commonly displays rounded grain boundaries. Hydrothermal altered monazite is typically Th-depleted and LREE-dominated, commonly containing quartz–feldspar inclusions and occurring in association with hydrothermal minerals. Inclusion-hosted monazite shows distinct compositional boundaries and characteristic REE signatures, with relatively elevated middle-REE signals, suggesting early encapsulation rather than late-stage replacement. Similar micro textures and comparable La/Ce ratios observed in both upstream bedrock and downstream sediments support an orogen-derived provenance for monazite in the Zhuoshui River system. Two compositional clusters in La/Ce further imply at least two source regions, tentatively linked to metamorphic source rocks in the Central Range and the Hsuehshan Range. Ongoing U–Th–Pb geochronology using laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS) will provide independent temporal constraints. These data will strengthen the proposed classification and provenance interpretations, clarifying sediment transport pathways in the Zhuoshui River.

How to cite: Yang, P.-C. and Chen, Y.-H.: Classification and Provenance of Monazite in the Zhuoshui River System, Taiwan, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16249, https://doi.org/10.5194/egusphere-egu26-16249, 2026.

EGU26-16463 | Orals | TS1.5

Tectono-Thermal Evolution of the Laojunshan Gneiss Dome in Yunnan, China: Constraints from Multi-Mineral Deformation and Composition 

Yun Tian, Shuyun Cao, Lefan Zhan, Jianhua Liu, Dingkui Zhou, Qingsong Li, and Lirong Tao

Gneiss domes are typical tectonic types related to deep crustal exhumation, and their polyphase superimposed deformation characteristics make them ideal natural laboratories for studying deep crustal exhumation processes. The Laojunshan gneiss dome in Yunnan, China, lies at the junction of the Tethyan and Circum-Pacific tectonic domains, as well as the boundary between the South China Block and Indochina Block. Its tectonic setting, deep crustal tectono-thermal evolution and exhumation history are closely linked to the kinematic evolution of the two blocks, making it a key site for investigating the Tethyan tectonic domain’s spatiotemporal evolution and inter-block interactions. Based on systematic field investigations combined with microstructural analysis, stress field inversion, electron backscatter diffraction (EBSD) analysis, geochemical and geochronological analyses, significant findings on the dome’s exhumation-related tectono-thermal evolution are obtained. The Laojunshan tectonic units comprise a core dominated by high-grade metamorphosed-deformed rocks and granites, an arcuate detachment fault system, and a sedimentary cover. Regional stress field inversion reveals two distinct regimes (compressional and extensional), with the latter predominant and radially distributed, reflecting late exhumation tectonics. EBSD analysis of major exposed minerals indicates the core underwent high-temperature plastic deformation (620–710 °C). Mylonite parameters (fractal dimension, differential stress) in the detachment fault zone reflect transitions between high and medium-high temperature deformation. Epidote EBSD constrains late exhumation P-T conditions to 350–500 °C, which, combined with geochemical data, divides late exhumation into three stages: deep compression, uplift transition and shallow extension. Geochronological data show the Caledonian (445–420 Ma) as the main formation period of granitic gneiss protolith (synchronous with coeval magmatism), core leucogranite emplacement at 416–411 Ma, and metamorphic zircons in plagioclase constrain Indosinian high-temperature metamorphism and shortening deformation to 241–220 Ma. An exhumation model is proposed: the dome initiated with early Caledonian (445–420 Ma) regional extension and magmatism, followed by 420–410 Ma compressional orogeny, crustal thickening and anatexis. Indosinian (241–230 Ma) compression induced thrusting, folding and detachment faults. Yanshanian (144–80 Ma) extension and magmatism accelerated exhumation, and Cenozoic (33–21 Ma) strike-slip faulting drove rapid exhumation to the surface.

How to cite: Tian, Y., Cao, S., Zhan, L., Liu, J., Zhou, D., Li, Q., and Tao, L.: Tectono-Thermal Evolution of the Laojunshan Gneiss Dome in Yunnan, China: Constraints from Multi-Mineral Deformation and Composition, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16463, https://doi.org/10.5194/egusphere-egu26-16463, 2026.

EGU26-16837 | ECS | Orals | TS1.5

Shear zone nucleation by fluid-assisted heterogeneous nucleation recorded in texturally homogeneous eclogitized mafic granulites 

Serena Cacciari, Giorgio Pennacchioni, Enrico Cannaò, Giovanni Toffol, Marco Scambelluri, and Jörg Hermann

Shear zone nucleation in massive rocks commonly exploits pre-existing planar structures, whose presence and type control fluid availability and redistribution. While fluids are widely recognized as key triggers for metamorphic reactions and mineralogical transformations that influence rock rheology, the exact feedback processes between fluid-rock interactions, metamorphism and deformation remain enigmatic. In specific cases, traditional softening mechanisms (e.g. reaction-induced grainsize reduction, crystallization of weak minerals) do not apply or are insufficient to explain shear zone nucleation and strain localization, implying the existence of alternative processes.

Paired shear zones developed at the selvages of hydration haoles are a common product of fluid infiltration along hydrofractures, and are a source of information to investigate the rheological effects of the different reaction extents occurring during fluid percolation. Here, we investigate a suite of samples containing eclogitic clinozoisite-filled veins surrounded by omphacite-rich haloes. The sample set includes haloes (a) weakly affected by ductile deformation, preserving pristine metasomatic textures, and (b) displaying paired shear zones at their selvages (Pennacchioni, 1996). The eclogitic host rock foliation, consisting of garnet, clinozoisite, amphibole and omphacite, is only partially obliterated in the hydration halo by the metasomatic overprint, dominated by replacement of clinozoisite by omphacite. EDS major element and in-situ LA-ICP-MS trace element analysis suggests that fluid propagation caused recrystallization, changes in mineral proportions and (re)distribution of major and trace elements, forming a compositional gradient across the halo. Garnet and clinozoisite rims record the gradient with a progressive decrease in the Fe2+ content and a progressive increase in LREE and Fe3+ concentrations from the vein selvage towards the reaction front, respectively.

Electron backscatter diffraction (EBSD) maps provide evidence for (i) a constant omphacite grainsize across the haloes and at their boundaries in samples weakly affected by ductile deformation, suggesting that metasomatism does not produce textural gradients, (ii) development of very fine-grained monomineralic ribbons of omphacite along the shear zones, suggesting that omphacite is responsible for weakening and localized shearing, (iii) local orientation of these ribbons at 20-30° to the shear zone trace, defining C' bands, and (iii) random orientation of the fine grains. We interpret these observations as evidence for diffusion-assisted grain boundary sliding (GBS) and creep cavitation as the main deformation mechanism active along the shear zones, and for heterogeneous nucleation of very fine-grained omphacite within fluid-filled cavities formed during GBS.

We conclude that, when metasomatic reactions do not directly result in textural gradients (e.g. grainsize decrease) traditionally considered responsible for softening at the propagation front (i.e. halo boundary), shear zones may develop by heterogeneous nucleation of fine grains during fluid-assisted GBS, which further fosters grainsize-sensitive deformation sustaining strain localization within fluid-rich domains.

[1] Pennacchioni, 1996. Journal of Structural Geology, 18, 549-561

How to cite: Cacciari, S., Pennacchioni, G., Cannaò, E., Toffol, G., Scambelluri, M., and Hermann, J.: Shear zone nucleation by fluid-assisted heterogeneous nucleation recorded in texturally homogeneous eclogitized mafic granulites, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16837, https://doi.org/10.5194/egusphere-egu26-16837, 2026.

EGU26-17135 | Posters on site | TS1.5

Texture-controlled hydrothermal dolomitization experiments to investigate interface kinetics and pore-scale transport 

Nicolas Beaudoin, Kanchana Kularatne, Stephen Centrella, Benjamin Lefeuvre, Pascale Sénéchal, Matthieu Mascle, Souhail Youssef, and Fadi Henri Nader

Dolomitization is a key diagenetic process that reorganizes porosity and permeability in carbonate rocks, yet the coupling between interface kinetics and transport heterogeneity remains poorly constrained. We performed time-resolved hydrothermal dolomitization experiments on oolitic limestone and chalk to test how carbonate texture impacts the dynamics of replacement fronts. Pseudo 4D micro-CT, along with SEM, EBSD and microprobe analyses reveal that the mechanism of dolomitization is depending on the texture and on the chemistry of the fluid. We studied oolitic limestone, chalk and carrara marble, three rocks with different porosity and permeability. In both oostone and chalk, dolomite rims propagate rapidly and produce wavy reaction fronts, witnessing a progressive replacement inward rather than along pore-connected pathways, unlike in the carrara marble. However, mass-balance calculation of the fluid rock interaction returns similar mass and volume loss independently of the texture, suggesting that the chemistry of the fluid controls the reaction. This is consistent with the produced dolomite grain size, who follow a similar distribution law regardless the texture, suggesting some self-organization during the replacement controlled by the fluids. Roughness characterization of the front shows that in oostone and carrara marble, the scaling law of the front follows a Brownian Motion (H=0.5), while it shows a persistent behaviour in the chalk (H=0.8 to 0.6). This suggests that the expression of the replacement process is governed by random distribution of heterogeneities in some cases, following the interface coupled dissolution precipitation model, but that there is a memory effect in other cases. In this study, the memory effect can be related mechanical processes such as local microfracturing, suggesting a potential role of local pressure on replacement. We propose that the shape of the front is governed by the rate of the front propagation, as if the latter is fast like in chalk, the mass transfer becomes less efficient to compensate the volume change, and some local overpressure may appear to drive the reaction propagation. This rate of front propagation appears to be affected by both initial grain size and pore size homogeneity.

How to cite: Beaudoin, N., Kularatne, K., Centrella, S., Lefeuvre, B., Sénéchal, P., Mascle, M., Youssef, S., and Nader, F. H.: Texture-controlled hydrothermal dolomitization experiments to investigate interface kinetics and pore-scale transport, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17135, https://doi.org/10.5194/egusphere-egu26-17135, 2026.

EGU26-18428 | ECS | Orals | TS1.5

The formation of the Münchberg Massif: New insights from petrology and chemistry of its serpentinite occurrences. 

Maximilian Hasch, Peter Klitzke, Meike Bagge, Nikola Koglin, and Christian Ostertag-Henning

Serpentinization is a hydration process that forms distinct serpentine minerals depending on the pressure and temperature conditions prevailing during the fluid-rock reaction. The chemistry and petrology of serpentinite rocks provide constraints on the protolith composition and on the tectonic setting of serpentinization through insights of pressure and temperature conditions.

The Münchberg Massif is a stack of four tectonic nappes of different metamorphic grade, which were emplaced during the Variscan Orogeny. Within the lowermost Prasinit-Phyllit-Serie, several serpentinite bodies are intercalated. Understanding the formation of these serpentinites will add further insights into the tectonic development of the Münchberg Massif.

We present new petrological and chemical data of serpentinites from ten locations along the southeastern margin of the Münchberg Massif, as well as at two locations in the western region of the Massif. The samples are dominated by the serpentine minerals lizardite in the western region and antigorite along the southeastern margin. Furthermore, significant differences in the degree of serpentinization and tectonic strain were observed between the two regions. The petrological and chemical characteristics of the samples indicate distinct protolith material and serpentinization setting. We propose that the protoliths of the western and southeastern serpentinites originated from different structural positions within, or adjacent to, a subduction zone. These findings provide new constraints on the tectonic assembly and metamorphic evolution of the Münchberg Massif.

How to cite: Hasch, M., Klitzke, P., Bagge, M., Koglin, N., and Ostertag-Henning, C.: The formation of the Münchberg Massif: New insights from petrology and chemistry of its serpentinite occurrences., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18428, https://doi.org/10.5194/egusphere-egu26-18428, 2026.

EGU26-19908 | ECS | Orals | TS1.5

Fault-related fluid circulation in the seismically active Irpinia region (southern Italy): insights from fluid inclusions and calcite veins 

Filippo Zummo, Antonio M. Alvarez-Valero, Andrea Billi, Dario Buttitta, Gabriele Carnevale, Barbara Marchesini, Ivana Pibiri, Rosa Sinisi, Luca Smeraglia, Antonio Caracausi, Fabrizio Agosta, and Michele Paternoster

The analysis of fault-related mineralization, with particular emphasis on fluid inclusions (FIs) trapped in syn-kinematic minerals, provides crucial insights into fluid circulation modality and fluid–rock interactions, so furnishing new tools to investigate the relationship between fluids and active tectonic. This study investigates the genesis, microstructural characteristics, and geochemical signatures of calcite veins associated with dip-slip faults in the Irpinia region (southern Apennines, Italy), a seismically active area located very close to the epicentral zone of the 1980 Mw 6.9 Irpinia earthquake. A comprehensive approach combining field observations, petrographic and microstructural analyses, fluid inclusion microthermometry, and geochemical profiling based on isotopic (δ¹³C and δ¹⁸O) and rare earth element (REE+Y) data reveals that the calcite veins precipitated from low-salinity H₂O–NaCl fluids, derived from the mixing of shallow and deep groundwater. These fluids, rich in CO₂ and coming from deep crustal reservoirs (8–12 km), migrated episodically through fault zones and were modified by mixing with post-depositional fluids produced during carbonate diagenesis, under varying thermal conditions (100–320 °C). Our study also proposes a computational model that reconstructs the isotopic evolution of the mineralizing fluids, capturing the sequential processes of fluid equilibration with dolostones, interaction with aquifer waters, and CO₂ degassing prior to calcite precipitation forming the mineralization. The good agreement between model predictions and measured isotopic data demonstrates the robustness of the model and highlights the dynamic fluid mixing processes within the fault zone. Furthermore, these findings highlight the role of episodic fluid migration, driven by fault-valve processes, in promoting calcite oversaturation and precipitation during seismic events. The integration of structural, geochemical, and modelling data refines our understanding of CO₂-rich fluid ascent, fault-related mineralization, and their link to fluid–rock interaction processes. This multidisciplinary approach offers new insights into fault mechanics and seismo-genesis, with implications for seismic hazard assessment and geochemical monitoring in active fault systems

How to cite: Zummo, F., Alvarez-Valero, A. M., Billi, A., Buttitta, D., Carnevale, G., Marchesini, B., Pibiri, I., Sinisi, R., Smeraglia, L., Caracausi, A., Agosta, F., and Paternoster, M.: Fault-related fluid circulation in the seismically active Irpinia region (southern Italy): insights from fluid inclusions and calcite veins, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19908, https://doi.org/10.5194/egusphere-egu26-19908, 2026.

EGU26-22277 | Posters on site | TS1.5

Mechanisms of Micritization Revealedby Petrography, Mg/Ca and Sr/Ca Ratios of the Carbonate Sediments of theArabian (Persian) Gulf, Abu Dhabi 

Almog Ash, Boaz Lazar, Adi Torfstein, Gilad Antler, Tianyu Cao, Tanya Rivlin, Mohammad Alsuwaidi, Sadoon Morad, and Mordechai Stein

The solidity and porosity of calcium carbonate rocks are of major interest for oil-reservoir
evaluation, groundwater flow studies, and civil engineering applications. Micritization—an
early diagenetic process that converts carbonate shells and skeletal grains into
microcrystalline carbonate—significantly affects these rock properties, yet its underlying
mechanisms remain poorly constrained. The coastal environments of Abu Dhabi provide
natural laboratories for studying micritization, as they are modern analogues of the low-angle
carbonate ramps that were widespread in epeiric seas throughout much of the geological past.
In this study, we investigate calcium carbonate muds and associated pore waters from a range
of depositional environments, including mangroves, tidal channels, sabkhas, and offshore
settings, to better understand the processes controlling micritization. We apply an integrated
approach combining sedimentological, mineralogical, and geochemical methods. Preliminary
results indicate that the carbonate mud is predominantly composed of aragonite, with minor
amounts of low magnesium calcite. Boring intensity increases with depth, particularly in
tidal-channel environments, and is closely associated with physical erosion by endolithic
fauna. In contrast, crystal morphologies observed in sabkha sediments suggest that chemical
precipitation processes are more dominant in these settings.
Trace element systematics reveal that micritization is accompanied by systematic changes in
Sr/Ca and Mg/Ca ratios. In all tested environments, grain size reduction (i.e., micritization) is
associated with a significant increase in Mg/Ca, while Sr/Ca is much less sensitive to the
same process. While both Sr/Ca and Mg/Ca are incorporated within the diagenetic aragonite
lattice according to their respective partition coefficients, Mg/Ca ratios are strongly increased
by adsorption during micritization-related grain size changes. The decoupling of Mg and Sr
during the micritization process may provide new constraints on the question of the
mechanism of micrite formation.

How to cite: Ash, A., Lazar, B., Torfstein, A., Antler, G., Cao, T., Rivlin, T., Alsuwaidi, M., Morad, S., and Stein, M.: Mechanisms of Micritization Revealedby Petrography, Mg/Ca and Sr/Ca Ratios of the Carbonate Sediments of theArabian (Persian) Gulf, Abu Dhabi, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22277, https://doi.org/10.5194/egusphere-egu26-22277, 2026.

As the key mechanism of shallow earthquakes, the fault stick-slip behavior is usually explored under the assumption of constant normal stress. However, dynamic natural processes (tides, far-field earthquakes, etc.) and human activities (blasting, water injection, mining, etc.) generate periodic stress disturbances in the fault zone. So far the coupled results of fault seismic slips under variable normal stress are poorly understood.

We performed laboratory direct shear tests on saw-cut granite joints under constant and cyclic normal stress (σn), considering the role of load point velocity (Vlp), normal stress oscillation amplitude (ε) and normal stress oscillation frequency (f). Under constant normal stress, the joint exhibits a spontaneous stick-slip phenomenon for different Vlp. The shear stress drops and recurrence timespans of stick-slip events are reduced with faster Vlp. Under equivalent σn level, the cyclic σn weakens the frictional strength when Vlp is small and enhances the strength when Vlp is large. As ε grows, the joint slip style switches from regular stick-slip to chaotic slip, and eventually to compound stick-slip. The frictional strength is first increased and later weakened. In respect to effect of f: when f is small, one σn cycle can produce several stick-slip events. When f is medium, the period of the stick-slip event is equal to the cyclic σn period. For further increase of f , the recurrence period of stick-slip events becomes double the cyclic σn period. The frictional strength is decreasing or increasing at the critical point for frictional resonance.

The improved spring-block model equipped with rate-and-state friction framework matches the lab observations satisfactorily. Especially, the introduction of a stiffness response coefficient (Ψ) allows the model to reflect realistic fault frictional behavior, where shear stiffness varies with σn. A new parameter Θ is defined whose symbol (+ or -) directly determines the compression/relaxation status of the spring, and satisfactorily explains transitions in shear stress trends. Comparative analysis with the conventional Linker-Dieterich model highlights the improved physical consistency of our new approach, particularly in preserving the physical interpretation of the state variable, θ. The model also demonstrates that under large σn disturbances, a frictional system can effectively exhibit stick-slip behavior even in the velocity-strengthening scope. More importantly, the modeling implies that fast slip events greatly reduce the contact density of the fault interface. The contact state of the stick-slip joint/fault cannot be judged solely by σn. The contact area during the shear process is determined by both, the real-time σn level and the state variable θ.

How to cite: Tao, K. and Konietzky, H.: Experimental and modeling insights into fault stick-slip behavior under dynamic normal stress condition, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2318, https://doi.org/10.5194/egusphere-egu26-2318, 2026.

EGU26-3420 | ECS | Posters on site | TS1.8

How an extensional pull-apart basin modulates fault slip and earthquake rupture on the Main Marmara Fault 

Deborah Osei-Tutu, Eyup Sopaci, and Luca Dal Zilio

Pull-apart basins introduce extensional bends and strong along-strike heterogeneity into otherwise strike-slip systems, potentially altering slow slip, earthquake nucleation, and multi-segment rupture. The Princes Islands segment of the Main Marmara Fault (MMF) hosts a ~30-40 km pull-apart basin within the Marmara seismic gap south of Istanbul, where geodetic and geological observations suggest partial unlocking and complex rupture behavior. Yet the mechanical role of this extensional geometry in controlling fault slip and rupture remains poorly constrained. We perform three-dimensional quasi-dynamic simulations using PyQuake3D (Tang et al., 2025) to quantify the impact of the Princes Islands pull-apart basin on interseismic loading, slow-slip transients, dynamic rupture propagation, and earthquake recurrence along the MMF. We model a continuous fault surface with variable dip, bends, and segmentation, and prescribe depth-dependent effective normal stress, spatial frictional contrasts, and stress heterogeneity representative of extensional basin environments, guided by published geophysical constraints. Our results show that the basin exerts a first-order control on slip style and rupture outcomes through the competition between geometric unclamping, frictional heterogeneity, and stress structure. Extensional bends favor localized unlocking and recurrent aseismic or slow-slip episodes, which in turn modulate where dynamic ruptures nucleate. At the event scale, the basin can behave either as a rupture barrier or a rupture accelerator: in many realizations, ruptures do not continue smoothly across the basin but instead produce triggered seismicity via static stress transfer and re-nucleation near segment boundaries. Stress concentrations at geometric transitions primarily govern nucleation locations, while frictional contrasts regulate rupture persistence and arrest. These findings highlight that explicitly representing extensional fault structures is critical for assessing multi-segment rupture potential and time-dependent seismic hazard on the MMF near Istanbul.

 

Tang, R., Gan, L., Li, F., & Dal Zilio, L. (2025). PyQuake3D: A Python tool for 3‐D earthquake sequence simulations of seismic and aseismic slip. Journal of Geophysical Research: Machine Learning and Computation, 2(4), e2025JH000871.

How to cite: Osei-Tutu, D., Sopaci, E., and Dal Zilio, L.: How an extensional pull-apart basin modulates fault slip and earthquake rupture on the Main Marmara Fault, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3420, https://doi.org/10.5194/egusphere-egu26-3420, 2026.

EGU26-3472 | ECS | Orals | TS1.8

Spontaneous complexity in the dynamics of slow laboratory earthquakes. 

Giacomo Pozzi, Giuseppe Volpe, Jacopo Taddeucci, Massimo Cocco, Chris Marone, and Cristiano Collettini

Rock deformation experiments play a key role in our understanding of earthquake physics and friction constitutive laws. These laws commonly describe the response of analogue laboratory faults as a simple and homogeneous system, without accounting for the spatial-temporal evolution of structures in the sample. However, increasing experimental evidence suggests that slip instability is closely tied to heterogeneity, complex rheologies, and inhomogeneous boundary conditions. To address this, we designed a novel transparent setup to observe real-time deformation, track the spatial-temporal evolution of shear fabric, and document unstable slip in experimental faults. Our video documentation reveals that the progressive development of fault fabrics results in heterogeneous but not random stress redistribution. We show that stress and structural heterogeneities play a key role in the nucleation, propagation, and arrest of slip instabilities, raising questions about the robustness of scaling laboratory frictional laws to nature.

How to cite: Pozzi, G., Volpe, G., Taddeucci, J., Cocco, M., Marone, C., and Collettini, C.: Spontaneous complexity in the dynamics of slow laboratory earthquakes., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3472, https://doi.org/10.5194/egusphere-egu26-3472, 2026.

EGU26-4626 | Posters on site | TS1.8

Fluid-Driven Injection and Pressurization of Clay-Rich Gouge in the Yangsan Fault: Implications for the Long-Term Seismic Cycle 

Chang-Min Kim, Sangwoo Woo, Jiah Lee, and Jiwoong Choi

Elucidating fault zone processes during long-term seismic cycles is critical for mitigating earthquake hazards in intraplate regions. We investigated the hydro-mechanical evolution of a strike-slip branch of the Yangsan Fault, SE Korea, which bounds Triassic and Jurassic granites. By integrating multiscale observation with high-velocity rotary shear experiments and XRD, we characterized the fault architecture, which consists of a <35 m thick damage zone surrounding a <1 m thick core. The core contains breccia and foliated gouge rich in clay minerals (43 wt.%), specifically dominated by illite (21.2 wt.%) and smectite (13.3 wt.%). Shear experiments on the foliated gouge revealed a consistently low friction coefficient (μss<0.17). Notably, instantaneous flash dilation of the mixed smectite/illite gouge was observed at seismic slip rates (1.3 m/s) when total displacement exceeded ~5 m. Microstructural cross-cutting relationships indicate a distinct sequence of events: (1) vigorous injection of pressurized fluids from wall rocks into the densely packed, low-permeability gouge directly; (2) precipitation of fibrous calcite veins along foliation planes and perpendicular to the Y-shear direction; and (3) subsequent injection of fluidized gouge material into the damaged wall rock. These observations suggest that cyclic coseismic and aseismic faulting occurred following the low-temperature formation of expanding clay minerals. We conclude that the dynamic interplay between fluid pressurization and the fluidization properties of clay gouge acts as a primary driver of mechanical instability, playing a key role in the long-term seismic evolution of intraplate granitic fault zones.

How to cite: Kim, C.-M., Woo, S., Lee, J., and Choi, J.: Fluid-Driven Injection and Pressurization of Clay-Rich Gouge in the Yangsan Fault: Implications for the Long-Term Seismic Cycle, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4626, https://doi.org/10.5194/egusphere-egu26-4626, 2026.

EGU26-4788 | ECS | Posters on site | TS1.8

Seismic Fault Identification Based on Vision Transformer 

Haoran Pei and Guangzhi Zhang

To address the limitations of traditional convolutional neural networks (CNNs) in seismic fault identification—such as restricted local receptive fields, limited capability for modeling long-range structural correlations, and low sensitivity to small or subtle faults—this study proposes a seismic fault identification framework based on a Vision Transformer (ViT) architecture combined with self-supervised pretraining and transfer learning. Self-supervised pretraining is first conducted on large volumes of unlabeled three-dimensional seismic data to learn general representations of geological structures, thereby reducing the dependence on manually labeled samples. The pretrained ViT model is subsequently transferred to the fault identification task and systematically compared with a conventional U-Net architecture. Experiments on a publicly available synthetic seismic dataset show that the ViT-based model achieves improved fault localization accuracy, spatial continuity, and robustness to noise compared to U-Net. Application to real 3D seismic data from an oilfield further demonstrates that the proposed method is capable of detecting a larger number of small-scale faults with enhanced structural continuity, highlighting its applicability in structurally complex settings. The results suggest that Transformer-based global modeling provides an effective alternative for automated seismic fault interpretation.

How to cite: Pei, H. and Zhang, G.: Seismic Fault Identification Based on Vision Transformer, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4788, https://doi.org/10.5194/egusphere-egu26-4788, 2026.

EGU26-6156 | ECS | Orals | TS1.8

Hydraulic control of the foreshocks and mainshock of the 2017 Valparaiso earthquake in central Chile 

Carlos Peña, Leoncio Cabrera, Jesús Muñoz-Montecinos, Sergio Ruiz, and Oliver Heidbach

Slow-slip events (SSEs) are a well-known mode of aseismic deformation in subduction zones. Seismological and geological studies further suggest that SSEs enhance fault-zone permeability, enabling fluid migration from overpressured oceanic crust into the plate interface. However, it remains unclear whether the resulting pore-pressure changes dominate stress transfer and promote the commonly observed increase in seismicity during SSEs and, although less commonly, the occurrence of larger megathrust earthquakes. Here, we investigate the impact of an SSE that occurred three days before the 2017 Mw 6.9 Valparaíso earthquake in central Chile. We use a forward 4D hydromechanical (poroelastic) model and compare the resulting spatial stress changes with a high-resolution seismicity catalog of the foreshock sequence.

We simulate the SSE by prescribing a geodetically inferred slip distribution on the fault interface and assume an overpressured oceanic crust, together with transient permeability enhancement due to SSE-induced local fracturing of the plate interface. We compute stress transfer driven by these pore-pressure changes along the plate interface and compare the results with widely used models that consider elastic stress changes only. Our results show that fluid migration into the plate-interface zone generates stress changes of ~1–10 MPa, overwhelmingly dominated by pore-pressure variations. The largest stress (and pore-pressure) changes spatially correlate with zones of increased seismicity, repeating earthquakes, and the mainshock. In contrast, the elastic-only scenario produces stress changes that are two to three orders of magnitude smaller and shows a much weaker spatial correspondence with the observed seismicity.

Our modeling results indicate that transient permeability enhancement during SSEs enables fluid redistribution that fundamentally controls stress transfer along the plate interface. We conclude that pore-pressure changes exert first-order control on earthquake precursors in subduction zones, offering a physical explanation for foreshock clustering and the triggering of large earthquakes during SSEs. These findings highlight the importance of incorporating fluid–rock interactions in models of seismic hazard and earthquake nucleation.

How to cite: Peña, C., Cabrera, L., Muñoz-Montecinos, J., Ruiz, S., and Heidbach, O.: Hydraulic control of the foreshocks and mainshock of the 2017 Valparaiso earthquake in central Chile, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6156, https://doi.org/10.5194/egusphere-egu26-6156, 2026.

EGU26-9583 | ECS | Posters on site | TS1.8

Fluid induced fault slip behavior: frictional healing vs velocity dependence of friction 

Luca Coppola, Giuseppe Volpe, Carolina Giorgetti, Giacomo Pozzi, Christopher Wibberley, Frédéric Bourgeois, and Cristiano Collettini

Fluid-induced fault reactivation and associated seismicity is a critical process in reservoir exploitation and emerging geo-energy activities such as Carbon Capture and Storage (CCS), Enhanced Geothermal Systems (EGS) and wastewater disposal. During fluid injection, the fault stress state progressively approaches the failure criterion τ = (σₙ - Pf) * µ + C , where τ is shear stress, σₙ normal stress, Pf fluid pressure, µ friction, and C cohesion. Once the stress state reaches the failure envelope, faults may reactivate either seismically or aseismically. However, the mechanisms governing aseismic versus seismic fault reactivation during fluid injection remain debated.

Previous laboratory studies suggest that this seismic vs. aseismic deformation may be influenced by fault frictional properties influenced by mineralogy, fault zone structure, stress state, and injection rate, yet the relative contribution of these factors remains unclear. To address this issue, we present an experimental study on binary and ternary fault gouges with variable fractions of quartz, calcite, and illite. These are minerals found along faults zones and within reservoir rocks commonly exploited for geo-energy applications.

For each mineralogical composition, two experimental datasets were acquired. In the first dataset, we performed slide–hold–slide and velocity-step tests to measure friction, frictional healing and the velocity dependence of friction. In the second dataset, we investigated fault slip behavior during fluid pressure-induced reactivation at three different stress states.

The frictional properties reveal a pronounced contrast between granular and platy phyllosilicate-rich gouges. Granular materials exhibit high friction (µ ≈ 0.6), positive frictional healing, and low a–b values, indicating velocity-weakening and potentially seismogenic behavior. In contrast, illite-rich gouges (illite > 40%) display low friction (0.28 < µ < 0.4), low to negative healing, and strongly positive a–b values, indicative of velocity-strengthening and aseismic behavior. Duringfluid injection induced-reactivation, granular-rich gouges reactivate through an exponential increase in slip velocity, mimicking seismic-like instability. Conversely, illite-rich gouges reactivate through aseismic but accelerated creep that does not evolve into dynamic failure.

Notably, reactivation in granular gouges is abrupt and occurs at stress states well above the predicted failure envelope, whereas in illite-rich gouges reactivation is gradual and occurs at or before the predicted failure envelope. In addition, at constant illite content, quartz-rich gouges reactivate faster than calcite-rich fault gouges.

The integration of these results suggests a conceptual framework in which fluid-induced fault reactivation is governed by the interplay between frictional healing and rate dependence, with mineralogy exerting a first-order control. In granular gouges, strong healing dominates the the fluid induced reactivation process, leading to delayed but abrupt fault reactivation that can overcome the stabilizing slight rate-strengthening effect, promoting an exponential acceleration under fluid pressurization. In contrast, in phyllosilicate-rich gouges, weak or negative healing combined with a marked rate strengthening behavior stabilizes slip, favoring continuous aseismic creep.

This framework demonstrates that the balance between healing and rate dependence, strongly linked to fault mineralogy, governs whether fluid-induced fault reactivation produces seismic slip or aseismic creep.

 

How to cite: Coppola, L., Volpe, G., Giorgetti, C., Pozzi, G., Wibberley, C., Bourgeois, F., and Collettini, C.: Fluid induced fault slip behavior: frictional healing vs velocity dependence of friction, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9583, https://doi.org/10.5194/egusphere-egu26-9583, 2026.

EGU26-9842 | ECS | Posters on site | TS1.8

The role of seamounts, fluids, and normal faults in slow slip regions: seismological insights from the northern Hikurangi margin 

Amy Woodward, Ian Bastow, Rebecca Bell, Laura Wallace, Katrina Jacobs, Stuart Henrys, Bill Fry, Thomas Merry, Victoria Lane, Laurene Ville, Phoebe Houldsworth-Bianek, and Luke Broadley

At the northern Hikurangi margin, Aotearoa New Zealand, slow slip events (SSEs) recur every 6-24 months to ~30 km depth. While shallow SSEs (0-10 km) are well-studied offshore, the deeper portion (10-30 km) remains poorly understood, limiting insight into SSE initiation. In Woodward et al. 2026 we investigate the relationships between newly resolved SSEs and seismicity. We combine passive seismological, geodetic, geochemical and seismic reflection data to analyse the relationships between seismicity and slow slip events, and the mechanisms that invoke them. Using time-dependent inversions, we resolve two small SSEs (MW 6.2 and 6.4), one of which extends unusually deeply from 15 to 30 km depth. Using data from a dense onshore seismograph network, deployed directly above this deeper portion from December 2017 to October 2018, we construct a catalog of 3,071 high-quality earthquakes with hypocentral uncertainties ≤5 km, located with a 3-D velocity model and our new 1-D model. Focal mechanisms reveal numerous normal-faulting earthquakes, including some within the slab mantle. Seismicity distributions and normal-faulting earthquakes occur along vertically aligned pathways that link the subducting slab mantle to surface seeps, where fluids show mantle-derived signatures. We infer that normal faults form due to slab bending and localized uplift of subducting seamounts, which enhance plate interface roughness, damage the upper plate, and promote fluid migration. Landward of ~100 km from the trench, both surface seeps and normal-faulting mechanisms cease, coinciding with the downdip limit of shallow SSEs. Together, these results suggest that the Hikurangi margin’s rough subducting plate interface exerts strong control on forearc dewatering and SSE genesis.

How to cite: Woodward, A., Bastow, I., Bell, R., Wallace, L., Jacobs, K., Henrys, S., Fry, B., Merry, T., Lane, V., Ville, L., Houldsworth-Bianek, P., and Broadley, L.: The role of seamounts, fluids, and normal faults in slow slip regions: seismological insights from the northern Hikurangi margin, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9842, https://doi.org/10.5194/egusphere-egu26-9842, 2026.

EGU26-12718 | ECS | Orals | TS1.8

Investigating seismic and aseismic fault motion caused by the 2024-2025 Fentale dyke intrusions in Ethiopia 

Simon Orrego, Juliet Biggs, Sam Wimpenny, Weiyu Zheng, Lin Way, Martin Vallée, Raphaël Grandin, and Elias Lewi

The faulting caused by dyke intrusions provide a novel opportunity to study the way natural fault systems respond to time-varying changes to the stress field. The recent 2024-2025 Fentale-Dofen dyking episode in the northern Main Ethiopian Rift (NMER) offers a rare opportunity to investigate these processes, as the surface deformation was captured in unusually high spatial and temporal resolution by satellite radar. 

In our study, we combine Interferometric Synthetic Aperture Radar (InSAR) data from the COSMO-SkyMed satellite, high resolution Digital Elevation Model (DEM), with a catalogue of >150 relocated moderated-sized earthquakes (M4.5-6) to study the spatio-temporal evolution of seismic and aseismic fault slip linked to dyking in the NMER. We focus on an area ~15 km north of the tip of the dyke, where we find fault patches showing both repeated seismic and aseismic slip occurring in close proximity, associated with surface deformation of <13 cm in 3 months. We consider three possible mechanisms for the observed fault behaviour: (1) that this is normal mainshock-aftershock sequence on faults governed by rate-and-state friction, (2) that elastic stress perturbations from the ongoing dyke intrusions reloaded the fault patches, or (3) that elevated pore-fluid pressure caused transient reductions in effective normal stress on the faults. Using slip and stress modelling, we will test these hypotheses and quantify how much seismic/aseismic strain is accommodated by pre-existing and newly formed faults, as well as the relative contribution of seismic/aseismic strain to accommodating shallow crustal extension during the dyking episode.

These findings provide new constraints on fault mechanics and the interaction with magmatic processes in rifting environments, improving our understanding of dyke-induced seismicity and the evolving nature of faults with repeated earthquakes. 

How to cite: Orrego, S., Biggs, J., Wimpenny, S., Zheng, W., Way, L., Vallée, M., Grandin, R., and Lewi, E.: Investigating seismic and aseismic fault motion caused by the 2024-2025 Fentale dyke intrusions in Ethiopia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12718, https://doi.org/10.5194/egusphere-egu26-12718, 2026.

EGU26-12855 | ECS | Posters on site | TS1.8

Fluids and Creeping Faults: Insights From Local Earthquake Tomography of the Creeping Section of the North Anatolian Fault 

Joel Szrek, Romain Jolivet, Bernd Schurr, Dirk Becker, Patricia Martínez-Garzón, Jorge Jara, and Ziyadin Çakir

Aseismic slip plays a key role in earthquake dynamics, but we currently do not fully understand why some faults slide aseismically. Aseismic slip is largely influenced by the fault zone's frictional behaviour, by its material composition, the presence of fluids, the geometry of the fault, and the fault zone fabric. Recent research has focused on the material composition, and more specifically on the evolution of resistance to slip with slip speed for different types of rocks. Generally, faults with rate-weakening behavior tend to host earthquakes, while faults with rate-strengthening behavior accommodate stress through aseismic slip. However, even in rate-weakening materials, low effective normal stress, induced by high pore fluid pressure, makes it unlikely for a slip instability to reach the critical size needed to nucleate regular earthquakes. Hence, the presence of high pressure fluid within fault zones may explain the presence of shallow aseismic slip along faults. However, we lack direct evidence of the presence of fluids along various faults where aseismic slip has been identified.

We use data from a dense network of seismometers along the North Anatolian Fault Zone SEISMENET1 to investigate spatial changes in seismic velocity along the section hosting aseismic slip. This section slips aseismically since at least 1944 and is the epicentral region of the last two large earthquakes that have struck the area, namely the 1944 M7.3 Bolu-Gerede and the 1943 M7.6 Tosia-Ladik earthquakes. Using local earthquake tomography, we test for a possible presence of fluids in the fault zone and a damage zone surrounding the epicentral region of the 1943 and 1944 earthquakes.

Our network includes 5 broadband seismometers and 10 geophones deployed around the creeping section along a narrow swath paralleling the fault trace. In addition to data from these 15 temporary stations, seismic data from 5 permanent broadband stations were collected. The final dataset includes 24,756 P arrivals and 21,311 S arrivals from 2,272 earthquakes, with magnitudes ranging from Mw0 to Mw4. We use the simul2023 code2 to simultaneously determine the 3D structure of the shallow crust and relocate the earthquake hypocenters.

We find kilometer-scale shallow high vp/vs anomalies (values in range of 1.8 up to 1.95), consistent with a damage asymmetry aligned with the observed rupture directions of historical earthquakes, indicating long-term preferred rupture directions along this segment of the NAF. Additionally, the creeping section of the North Anatolian Fault is shown to correspond to a 30-km-long zone of vp/vs above 1.8, consistent with the presence of high pore fluid pressure within the fault zone. The findings provide compelling evidence that fluid processes, rather than fault zone rheology alone, significantly influence aseismic slip behavior along the NAF. Together, these results suggest a dynamic interplay between structural damage, rupture history, and fluid migration in controlling fault zone mechanics, with implications for improving seismic hazard assessment in creeping fault segments.

 

1https://geofon.gfz.de/waveform/archive/network.php?ncode=1O&year=2022

2https://doi.org/10.5281/zenodo.10695070

How to cite: Szrek, J., Jolivet, R., Schurr, B., Becker, D., Martínez-Garzón, P., Jara, J., and Çakir, Z.: Fluids and Creeping Faults: Insights From Local Earthquake Tomography of the Creeping Section of the North Anatolian Fault, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12855, https://doi.org/10.5194/egusphere-egu26-12855, 2026.

Understanding the physical mechanisms governing megathrust seismicity and the geodynamic feedback between the megathrust and the overriding accretionary wedge remains critical in subduction zone geophysics. The structural complexity of accretionary wedges—characterized by heterogeneous porosity, permeability, and fault networks—critically influences the configuration of pore fluid pressure and frictional properties along the megathrust interface. To investigate these interactions, we employ a fully coupled hydro-mechanical numerical model (Gerya, 2019) that simulates two distinct timescales within a single, consistent rheological framework. Our approach incorporates temperature-dependent dehydration reactions, including smectite-to-illite and zeolite-to-greenschist transitions, to evaluate how fluid production and migration evolve during both subduction and seismic processes. Additionally, we implement a dynamic fault-valving mechanism where reference permeability evolves transiently to mimic fracture-induced permeability enhancement during fast slip. The simulation follows a two-stage workflow: first, we conduct long-term wedge accretion modeling with adaptive time steps (10–500 years) using a higher stress tolerance to construct realistic wedge architectures. Subsequently, we switch to a rupture simulation mode by reducing the stress tolerance, allowing the adaptive time-stepping scheme to automatically resolve short-term seismic cycles (from days to years). This methodology successfully introduces the structural and hydrological complexity inherited from long-term geological evolution into the analysis of short-term megathrust slip behaviors. Results indicate that fast slip events preferentially initiate at the transition zones between low and high overpressure regions, whereas domains characterized by high pore fluid pressure ratios () predominantly host slow slip events. Furthermore, we find that hydraulic properties control the spatiotemporal stability of rupture nucleation: higher permeability promotes significant temporal pore pressure variability, resulting in scattered initiation depths, while lower permeability maintains stable pressure configurations, leading to spatially consistent rupture nucleation. We conclude that the long-term hydro-mechanical evolution of the wedge governs megathrust nucleation and slip segmentation. 

How to cite: Lin, C.-H. and Tan, E.: Hydro-Mechanical Modeling of Fluid-Regulated Deformation in Accretionary Wedges and Its Implications for Megathrust Slip, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12927, https://doi.org/10.5194/egusphere-egu26-12927, 2026.

Independent lines of seismic evidence suggest that pore fluid pressure at the depth range of episodic slow slip events (SSEs) may undergo periodic fluctuations synced with the SSE slip cycles.  Here we develop a numerical simulation framework that integrates the SSE model governed by the rate- and state-dependent friction with Bayesian data assimilation to optimize time-variable fault friction parameters, using constraints from the northern Cascadia GNSS time series.  We first conduct synthetic experiments to calculate surface displacement time series from the rate-state SSE model generated fault slip history with imposed Gaussian noise. Both frictional parameters, effective normal stress (normal stress minus pore pressure) and characteristic slip distance, converge to their true values in 5-10 iterations from the initial guesses that are 10-20% off from the true values, demonstrating the feasibility of the data assimilation framework. We then apply this framework to 2009-2020 GNSS time series that encompasses SSE cycles recorded at ~ 30 stations along the northern Cascadia subduction zone.  We use a GNSS time series of 1000 days (~3 SSE cycles) in each inversion run to fully resolve the temporal changes in stress or friction; longer time series will cause inversion convergence issues due to the system nonlinearity. Within an inversion run, we choose a sliding time window of 9 months for each optimization epoch, which is a trade-off that on one hand includes sufficient information for the prediction of fault slip in the next time step and on the other hand allows temporal distinctions between the inter- versus intra-SSE time periods. Our inversion results show clear cyclic fluctuations in the optimized characteristic distance and effective normal stress values during SSE cycles. Specifically, effective normal stress increases (pore pressure drops) during the intra-SSE period; effective normal stress decreases (pore pressure increases) during the inter-SSE period.  The pore pressure oscillation pattern is independent of whether the characteristic slip distance is time-invariant during data assimilation, but the converse does not hold. Our results are thus consistent with the proposed pore pressure build-up and release processes, i.e., fault-valve model, at the SSE depth range. 

How to cite: Liu, Y. and Zhang, W.: Fault-valve behavior during slow slip cycles constrained using Bayesian data assimilation for a Cascadia subduction fault slip model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13013, https://doi.org/10.5194/egusphere-egu26-13013, 2026.

EGU26-14122 | ECS | Posters on site | TS1.8

Fault state evolution governed by cumulative slip history. 

Joaquin Julve Lillo, Ake Fagereng, Jean-Paul Ampuero, Martijn van den Ende, and Giovanni Toffol

Given the significant risk that earthquakes pose to society, understanding the spatiotemporal evolution of slip rates on natural faults has been a central research objective over recent decades. Geological and geophysical observations indicate that fault slip is accommodated by multiple deformation mechanisms operating both on the fault plane and within the surrounding damage zone. At the outcrop scale, structures formed by seismic and aseismic slip commonly coexist within the same fault system, implying that fault displacement involves a combination of deformation processes controlled by mineral-specific rheology. At larger scales, however, these processes may be masked by the limited spatial and temporal resolution of geophysical and geodetic observations.

From a theoretical and experimental perspective, rate-and-state friction (RSF) laws have been widely used to explain unstable fault slip through velocity-weakening behaviour, in which fault strength decreases with increasing slip rate. In this framework, fault friction is governed by slip velocity and a single state parameter that evolves with time and slip, commonly expressed either through an aging law, where fault healing occurs primarily during stationary contact, or a slip law, where state evolution is driven by slip-dependent renewal of contacts. Because both formulations are typically expressed as local, slip-rate-dependent laws, the explicit role of cumulative slip history in controlling the fault state remains implicit.

To investigate the effect of cumulative slip history, we perform a suite of 3D quasi-dynamic simulations assuming a homogeneous distribution of rate-weakening frictional properties, in which fault slip is governed by a classical RSF formulation. By systematically decreasing effective normal stress from 50 to 10 MPa and explicitly rewriting the aging law in a slip-dependent, event-integrated form, we show that the well-documented transition from characteristic earthquake behaviour to deterministic chaotic slip (e.g., Rubin, 2008; Cattania, 2019; Barbot, 2019) is accompanied by a change in the role of the state variable. Specifically, state evolution becomes increasingly governed by cumulative slip history and slip-filtered healing, which inhibits convergence toward a unique healed state and results in incomplete state recovery between successive events. Importantly, this behaviour arises without prescribing any spatial heterogeneity in frictional properties or fault-zone structure.

These results have direct implications for the interpretation of fault kinematics. While regions where slip rates remain below the prescribed background velocity may persist constant over interseismic periods, the shear stress within those regions in models of low effective normal stress need not be stationary. Instead, shear stress can evolve significantly because of incomplete state recovery driven by cumulative slip history and slip-limited healing, leading to temporally heterogeneous mechanical behaviour despite stable kinematic expression.

References

Rubin, A. M. (2008). Episodic slow slip events and rate‐and‐state friction. Journal of Geophysical Research: Solid Earth, 113(B11).

Cattania, C. (2019). Complex earthquake sequences on simple faults. Geophysical Research Letters, 46(17-18), 10384-10393.

Barbot, S. (2019). Slow-slip, slow earthquakes, period-two cycles, full and partial ruptures, and deterministic chaos in a single asperity fault. Tectonophysics, 768, 228171.

How to cite: Julve Lillo, J., Fagereng, A., Ampuero, J.-P., van den Ende, M., and Toffol, G.: Fault state evolution governed by cumulative slip history., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14122, https://doi.org/10.5194/egusphere-egu26-14122, 2026.

EGU26-14191 | Posters on site | TS1.8

PolystyQuakes : what can we learn from the use of polystyrene as analogue to earthquakes? From small to large scale and vice versa. 

Audrey Bonnelye, Bastien Walter, Abraham Gouedar, and Delphine Faure-Catteloin

Laboratory investigations into the behavior of fault zones have been a significant focus in experimental rock mechanics over the past decades. Various approaches have been developed, ranging from analog models to testing natural samples in triaxial cells. The primary goal of the latter is to infer the physical mechanisms responsible for failure under realistic conditions encountered in natural settings, albeit on small sample sizes (e.g., centimeter scale). In contrast, analog modeling aims to replicate similar mechanical behavior by applying scaling laws to geometry and material properties. In the present study we aim at combining large scale experiments (meter scale) with small scale experiments (cm scale) in order to highlight the underlying physical mechanisms preceding the slip.

To address the spatial scale limitations of classical rock mechanics, we developed new experiments that bridge the gap between traditional rock mechanics and analog experiments. These experiments utilize the unique capabilities of the DIMITRI setup, a giant true-triaxial apparatus (1.5m × 1.5m × 1m). Due to the size of this experimental device, the maximum stress it can apply is limited to 2 MPa per principal stress. Consequently, we chose polystyrene as an analog for rocks. The low elastic properties of polystyrene slow down physical processes, enabling comprehensive observation of rupture phenomena, from initiation to failure arrest. Our objective is to investigate the interplay between different types of slip occurring along the interface.

In this study, we conducted stick-slip experiments on large-scale polystyrene blocks with a pre-cut surface area of 1.5 m². We applied shortening rates ranging from 1 to 10 mm/min. Our experiments successfully reproduced stick-slip behavior, allowing us to observe variations in frictional behavior along the interface and identify different types of slip, from slow slip to dynamic slip.

In parallel, we performed small scale experiments uniaxial stick slip experiments, under the same conditions than the previous, that we monitored with 2D X-ray radiography at high frequency (12Hz). Preliminary observations highlight density contrasts in the bulk material around the fault plane, offering insight into potential precursory signs of slip.

Therefore, this study including two scales of observation demonstrates the relevance of our material to study the physical mechanisms controlling various slip types occuring along the seismic cycle.

How to cite: Bonnelye, A., Walter, B., Gouedar, A., and Faure-Catteloin, D.: PolystyQuakes : what can we learn from the use of polystyrene as analogue to earthquakes? From small to large scale and vice versa., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14191, https://doi.org/10.5194/egusphere-egu26-14191, 2026.

EGU26-14725 | ECS | Orals | TS1.8

Fluid-induced aseismic slip and seismicity on a natural fault: insights from the FEAR1 experiment at BedrettoLab 

Aurora Lambiase, Men-Andrin Meier, Elena Spagnuolo, Mehdi Nikkhoo, David Marsan, Antonio Pio Rinaldi, Valentin Gischig, Paul Selvadurai, Massimo Cocco, Domenico Giardini, and Stefan Wiemer

Aseismic slip is increasingly recognized as a fundamental driver of earthquake nucleation, affecting the spatio-temporal evolution of seismicity, yet its direct observation remains rare due to limited strain measurements close to a natural fault system. Here, we present results from the 'FEAR1' experiment conducted at the Bedretto Underground Laboratory for Geosciences and Geoenergies (Switzerland), where we used fluid injections to activate a natural fault and fracture network in crystalline rock under in-situ stress conditions at ~1 km depth. This experimental setting is particularly well suited to investigate induced seismicity and the role of aseismic processes in fault activation, thanks to dense near- and on-fault strain, pressure, and seismic monitoring.

During several injections performed in FEAR1, we observed the activation of a steeply dipping, highly permeable fracture zone, which intersects a densely instrumented borehole. Hydraulic stimulations triggered seismicity (−4.9 < Mw < −2.3) that organized along a plane whose orientation is consistent with geological observations in boreholes cores, logs and on the laboratory tunnel wall. Simultaneously, high-resolution Fiber Bragg Grating strain measurements revealed progressive, irreversible tensile deformation localized near the fracture intersection with the monitoring borehole, reaching nearly 1000 µε over the course of the experiment.

Static elastic modeling demonstrates that the cumulative strain produced by the recorded earthquakes accounts for less than 1% of the observed deformation, indicating that fault slip was dominantly aseismic. The spatial and temporal evolution of seismicity shows systematic up-dip migration toward the strain concentration zone and the emergence of families of repeating earthquakes. The recurrence rate and cumulative slip of these repeaters correlate with the measured strain rate and strain, suggesting a scenario where seismic asperities are embedded within a creeping fault segment sustained by pore pressure stress perturbations.

Inversions of irreversible strain for simplified slip sources indicate a predominantly strike-slip mechanism consistent with the estimated local stress field, although trade-offs between source location, source dimension and slip direction highlight the limits of 1D strain observations. Our results provide direct experimental evidence for fluid-driven aseismic slip on a natural fault and demonstrate how microseismicity and repeaters can serve as indirect proxies for underlying slow deformation.

How to cite: Lambiase, A., Meier, M.-A., Spagnuolo, E., Nikkhoo, M., Marsan, D., Rinaldi, A. P., Gischig, V., Selvadurai, P., Cocco, M., Giardini, D., and Wiemer, S.: Fluid-induced aseismic slip and seismicity on a natural fault: insights from the FEAR1 experiment at BedrettoLab, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14725, https://doi.org/10.5194/egusphere-egu26-14725, 2026.

EGU26-14991 | Orals | TS1.8

Pore Fluid Pressure Effects on Friction and Fracture 

Ake Fagereng, Wenlu Zhu, Olivier Gagliardini, Thomas V. Schuler, and Francois Renard

Slip instabilities leading to earthquakes, landslides, and glacier surges may be triggered by high fluid pressures. On the other hand, high fluid pressures also suppress instability because of large nucleation length-scales in overpressured systems. We review geological, glaciological, and rock mechanical observations and highlight two key scales that control pore pressure induced frictional instabilities: (1) the length scale over which pore fluid overpressure is maintained, and (2) a time scale defined by relative rates of deformation propagation and pore fluid transport. These scales are also dependent on rheological regime, and we find three end-member regimes: (1) shallow and/or low temperature deformation where ambient stress is low, faults are close to frictional failure, and shear is easily delocalised; (2) deformation in a brittle and frictionally unstable regime (such as the crustal seismogenic zone), where planes are close to frictional failure and slip tends to localise; and (3) environments where viscous deformation is preferred over frictional, and hence bulk stress is low, frictional strength is high, and delocalisation dominant. In regimes 1 and 3, fluid-driven instabilities tend to be confined to local areas of overpressure, because deformation delocalises in the bulk and dilatant hardening prevents further propagation. In regime 2, however, slip tends to localise and it is potentially favourable for fluid-induced instabilities to grow, provided slip surfaces are sufficiently close to failure. These regimes also apply to glaciers, where viscous flow of ice competes with frictional sliding on the glacier base - here, interconnected overpressured water at the glacier base is a commonly invoked mechanism that promotes frictional instability. These concepts imply that fluid-driven frictional instabilities are only as large as the areas where fluid overpressured patches can be interconnected, and therefore highlight the key role of fluid pressure heterogeneity in determining whether fluid-induced instabilities can propagate.

How to cite: Fagereng, A., Zhu, W., Gagliardini, O., V. Schuler, T., and Renard, F.: Pore Fluid Pressure Effects on Friction and Fracture, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14991, https://doi.org/10.5194/egusphere-egu26-14991, 2026.

In subduction zones, the depth-dependent release of fluids from compaction and metamorphic dehydration reactions in hydrous lithologies plays a key role in modulating pore fluid pressure, fault strength, and slip behavior along the megathrust. The depth-distribution of fluid release is also the primary control on volatile fluxes through the forearc, and on the residual volatile content of the subducting plate. Here, we investigate the inventory and release of fluids from altered oceanic crust by low-grade dehydration reactions (~50-350 °C) at the Northern Hikurangi subduction zone, where slip on the outer (shallow) megathrust is accommodated almost entirely in frequent, large shallow slow slip events (SSEs).

Regional geophysical surveys and drilling during International Ocean Discovery Program (IODP) Expedition 375 show that the incoming plate of the Hikurangi Plateau carries a thick (>1.5 km) and extensively altered volcaniclastic sediment blanket characterized by an abundance of phyllosilicates (primarily Mg-smectite) and zeolite, and mineral-bound water contents as high as 14-16 wt.%, into the SSE source region. We quantify the distribution of fluid release from this sediment package by combining compaction trends to assess compactive water loss and thermodynamic phase equilibria models using sediment drill-core compositions to compute water release from dehydration reactions.

We find that: (1) compactive dewatering dominates in the outermost 15-20 km of the forearc, where temperatures remain too low (<100 °C) to drive dehydration reactions; and (2) a large volume (~5-8 wt.%) of mineral-bound water is released step-wise over the region spanning from ~30-90 km from the trench (corresponding to depths of 5-15 km below seafloor and temperatures of 150-260 °C), primarily from decomposition of zeolite and phllyosilicate phases. This contrasts with the behavior of Ca- and Na-smectites typically found in detrital marine sediments and altered volcanic ash, which undergo dehydration between 80-150 °C.

Because the majority of compactive dewatering precedes dehydration, mineral-bound water is released where porosity, permeability, and compressibility are reduced, maximizing the potential for excess pore pressure generation along and beneath the megathrust. The broad region of low-temperature metamorphic fluid release directly overlaps the slip zone of recurring SSEs, supporting the idea that dehydration - and associated elevated pore pressures and low effective normal stress - favor SSE as the prevailing mode of strain release on the plate interface. The presence of thick extensively hydrated oceanic crust and persistence of fluid production from clay dehydration to ~260 °C contrasts with other subduction zones, where low-T metamorphism is dominated by the transformation of Ca- and Na-smectites to illite by 120-150 °C. We speculate that this difference may offer an underlying explanation for the lack of a locked seismogenic zone at the Northern Hikurangi margin, whereas at other subduction margins, a lack of significant fluid production from dehydration in the 150-350 °C window may lead to a better-drained megathrust and promote stick-slip behavior.

How to cite: Saffer, D. and Smye, A.: Links between Low-T Dehydration and Recurring Shallow Slow Slip Events in the Northern Hikurangi Subduction Zone, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15863, https://doi.org/10.5194/egusphere-egu26-15863, 2026.

EGU26-16488 | ECS | Orals | TS1.8

Seismogenic width control on the dynamics and scaling of laboratory elongated ruptures 

Federica Paglialunga, Jean Paul Ampuero, and François Passèlegue

After an initial phase of circular expansion, very large earthquakes primarily grow horizontally, with their vertical extent limited by the seismogenic width of the Earth’s crust. This geometric evolution is accompanied by a transition in rupture dynamics from crack-like to pulse-like propagation. Such events are commonly referred to as elongated ruptures.

While classical models (f.e., Linear Elastic Fracture Mechanics (Freund, 1998)) successfully describe small to moderate earthquakes, they fail to capture the dynamics of large events. Recent theoretical and numerical work by Weng and Ampuero (2019) introduced a physical framework for elongated ruptures, which, although supported by numerical validation and natural observations, has yet to be experimentally validated.

To address this, we conducted 2D rupture experiments in a biaxial direct shear apparatus under unbounded and bounded conditions. The unbounded case corresponds to a uniform velocity-weakening interface, while the bounded case consists of an elongated velocity-weakening region adjacent to a wide velocity-strengthening zone, mimicking a seismogenic layer whose width is bounded by deep aseismic regions. This experimental model successfully reproduces confined elongated ruptures and reveals distinct propagation styles: crack-like ruptures under unbounded conditions and pulse-like ruptures under bounded conditions. This transition is also reflected in the temporal evolution of seismic moment: during the initial phase of propagation, seismic moment scales cubically with rupture duration, while after saturation of the seismogenic width, it transitions to a linear scaling, as expected for pulse-like ruptures.

Together, these observations highlight the role of the seismogenic layer in controlling rupture style and provide experimental support for the proposed theory of elongated ruptures.

How to cite: Paglialunga, F., Ampuero, J. P., and Passèlegue, F.: Seismogenic width control on the dynamics and scaling of laboratory elongated ruptures, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16488, https://doi.org/10.5194/egusphere-egu26-16488, 2026.

EGU26-17727 | Orals | TS1.8

Pore pressure change during nucleation and slip along experimental faults 

Nicolas Brantut, François Passelègue, and Pierre Dublanchet

Fluid pressure variations within fault zones impact fault strength and have the potential to produce detectable geophysical signals that can help characterise fault dynamics. One key process impacting fluid pressure is pore volume variations (dilation or compaction) due to stress changes and inelastic deformation. Slip-induced dilation and compaction have been thoroughly documented in laboratory experiments, but their impact on pore pressure has not. In nature, we expect slip to be associated with stress variations, and there might be cumulated effects of poroelastic and inelastic pore pressure changes. In order to document such effects, we conducted laboratory rock friction experiments where fluid pressure was monitored in situ during sequences of quasi-static loading followed by dynamic slip event. The simulated fault was a 30 degrees saw-cut in a Westerly granite cylinder, saturated with water, tested under triaxial conditions. The low hydraulic diffusivity of the rock made the fault and wall rock transiently undrained during deformation. During quasi-static loading with no fault slip, we observed pore pressure rises that we interpret as poroelastic closure of the fault. During dynamic slip events, pore pressure systematically dropped, approximately in proportion to the drop in normal stress. A large contribution to the pore pressure drop is interpreted as poroelastic opening of the fault. Prior to stick-slip events, we detected systematic pore pressure decreases by up to around 1 MPa, correlated to the occurrence of inhomogeneous slip along the fault. Slip nucleation, inferred by kinematic inversion of local strain gauge data, is linked to local slip magnitudes of the order of 1 to 10 µm, and appears to lead to inelastic dilation. A stability analysis of fault slip including dilatant and poroelastic effects shows that poroelastic coupling tends to compensate normal stress variations, leading to faults operating under mostly constant effective normal stress if conditions are undrained.

How to cite: Brantut, N., Passelègue, F., and Dublanchet, P.: Pore pressure change during nucleation and slip along experimental faults, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17727, https://doi.org/10.5194/egusphere-egu26-17727, 2026.

EGU26-18025 | Posters on site | TS1.8

Slip Rates on the Main Marmara Fault from Bayesian Inversion of Dense GNSS and InSAR Velocity Fields 

Émilie Klein, Estelle Neyrinck, Baptiste Rousset, Frédéric Masson, Ali Ozkan, Hakan Hasan Yavasoglu, Patrice Ulrich, Romain Jolivet, Cécile Doubre, Philippe Durand, and Marie-Pierre Doin

The Main Marmara Fault lies at the western termination of the North Anatolian Fault. While the North Anatolian Fault ruptured from its eastern termination to the Izmit segment over the 20th century through a westward‐propagating sequence of Mw ≥ 7 earthquakes, the underwater Marmara segment has not experienced a large earthquake in recent times. However, due to its proximity to the megacity of Istanbul, this segment represents one of the most hazardous fault systems in the Middle East. In particular, no historical earthquake has been identified on the Central Basin segment since at least 1766, potentially making it a major seismic gap.

To better assess seismic hazard along the Main Marmara Fault, we estimate the slip rate by jointly using a dense GNSS velocity field and four Sentinel-1 InSAR tracks. The GNSS velocity field consists of 111 measurements, including newly acquired densified sites along the northern shore of the Marmara Sea. The InSAR velocity field was processed automatically within the framework of the FLATSIM project, covering the period from October 2016 to April 2021. InSAR velocities are referenced to a Eurasia-fixed plate using the GNSS velocity field. We then perform a joint Bayesian inversion of slip rates using both datasets, allowing us to quantify uncertainties on the estimated slip rates.

Our results indicate that the Main Marmara Fault is predominantly creeping between longitudes 27.5 and 28.6, implying that the Central Basin segment is largely aseismic. Uncertainty estimates and forward modeling demonstrate that our datasets are capable of resolving slip behavior on this segment with good accuracy. However, the shallow portion of the Central Basin segment is still accumulating up to ~10 mm/yr of slip deficit, which could permit earthquakes of up to Mw 6.0 every few decades, similar to the 2025 sequence. West of longitude 27.5 and east of longitude 28.6, including the Prince Islands segment, the fault appears to be mostly locked down to 12 km depth. On the Prince Islands segment, close to Istanbul, the accumulated strain has the potential to generate an earthquake with Mw > 7.

How to cite: Klein, É., Neyrinck, E., Rousset, B., Masson, F., Ozkan, A., Yavasoglu, H. H., Ulrich, P., Jolivet, R., Doubre, C., Durand, P., and Doin, M.-P.: Slip Rates on the Main Marmara Fault from Bayesian Inversion of Dense GNSS and InSAR Velocity Fields, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18025, https://doi.org/10.5194/egusphere-egu26-18025, 2026.

EGU26-20370 | Posters on site | TS1.8

Seismic vs aseismic deformation in the Northern Apennines constrained from dense GNSS velocities 

Enrico Serpelloni, Riccardo Nucci, Giulio Poggiali, Mauro Buttinelli, Letizia Anderlini, Chris Marone, and Lauro Chiaraluce

The Upper Tiber Valley, in the Northern Apennines of Italy, is a key natural laboratory for investigating how continental extension is partitioned between seismic and aseismic deformation. Extension in this sector of the Apennines has been primarily accommodated by the Altotiberina Fault (ATF), a low-angle (~15°) normal fault that is mechanically unfavorable for elastic shear failure, and by a network of high-angle synthetic and antithetic faults in its hanging wall. While the ATF is characterized by persistent background micro-seismicity, the high-angle faults host larger historical earthquakes and frequent seismic swarms, likely induced by fluid circulation and elevated pore pressure. Since the study of Anderlini et al. (2016), the local GNSS network has been significantly densified within the framework of the Alto Tiberina Near Fault Observatory (TABOO-NFO). The updated dataset now better resolves a sharp ~3 mm/yr chain-normal interseismic velocity gradient across the Upper Tiber Valley, providing unprecedented constraints on how ongoing extension is distributed across the fault system. We use the new GNSS velocity field to reassess the relative contribution of low-angle versus high-angle faults to crustal deformation and to quantify the partitioning between seismic and aseismic slip. We apply a block-modeling approach that jointly estimates rigid block rotations and spatially variable interseismic coupling through a newly developed iterative inversion strategy. The model includes 3D geometries, discretized in triangular dislocation elements, of both the ATF and its antithetic structures, permitting assessment of distributed slip rates across the fault system. Preliminary results show that shallow locking on high-angle syn- and antithetic faults plays a first-order role in explaining the observed velocity gradient, whereas the ATF accommodates a significant fraction of extension through aseismic creep. These findings refine earlier interpretations and provide new insight into how low-angle normal faults can interact with steeper faults during the earthquake cycle.

How to cite: Serpelloni, E., Nucci, R., Poggiali, G., Buttinelli, M., Anderlini, L., Marone, C., and Chiaraluce, L.: Seismic vs aseismic deformation in the Northern Apennines constrained from dense GNSS velocities, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20370, https://doi.org/10.5194/egusphere-egu26-20370, 2026.

Shallow slow slip events have long been observed along the strike slip faults of the San Andreas fault system and are now increasingly observed on many other faults on Earth. Creep events are thought to episodically release a portion of the fault’s interseismic stress budget that has accumulated over the earthquake cycle. However, it is not known what portion of strain these events release, and what residual strain remains available to drive earthquake occurrence. Near-field surface creep measurements, like alignment arrays and creepmeters, are unable to constrain the depth of creep, meaning that is difficult to constrain the release of strain or stress in each creep event without additional assumptions. In this study, we use radar data from InSAR platforms to resolve the depth of creep during creep events along the Superstition Hills fault in Southern California. We mitigate atmospheric noise by stacking co-event interferograms and by using empirically derived covariance matrices in the modeling. We apply a new nonlinear dislocation modeling method that constrains the slip distribution to be elliptical at each point along the fault and uses field and creepmeter data as lower bounds on surface slip. Using this model, we compute the strain drop throughout the rupture. We apply this technique to the 2006, 2010, 2017, and 2023 aseismic ruptures in Envisat, UAVSAR, and Sentinel-1 data. Lastly, we compare the resulting strain drops to strain accumulation rates calculated from backslip, testing the hypothesis that shallowly released strain is equal to the strain applied from deep dislocations in the crust. Using only the creep events in the instrumental record, we find that interseismic slip rates on the SHF must be above 10 mm/yr to explain the observations, a result consistent with regional-scale block modeling. Our results have implications for the strength of faults, the expected modes of seismic moment release in the shallow crust, and for seismic hazard analyses near creeping faults.

How to cite: Materna, K. and Bilham, R.: Shallow Aseismic Slip and Stress/Strain Budgets on the Creeping Faults in the Imperial Valley, California, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21901, https://doi.org/10.5194/egusphere-egu26-21901, 2026.

EGU26-271 | Posters on site | TS1.6

A Local Seafloor Pressure Anomaly Potentially Triggered by Pore Water Migration during Ocean Current Meander 

Keisuke Ariyoshi, Akira Nagano, Takuya Hasegawa, Masaru Nakano, Hiroyuki Matsumoto, Chastity Aiken, Eiichiro Araki, Narumi Takahashi, and Takane Hori

Owing to the Dense Oceanfloor Network System for Earthquakes and Tsunamis (DONET) and borehole observatories, slow slip events (SSEs) have been detected in the shallow extension of the source region of the 1944 Tonankai earthquake (DONET-1). However, a localized seafloor pressure anomaly—characterized by uplift and subsidence at two DONET-1 stations in 2013—has yet to be reasonably explained.

In this study, we explore possible source models for this pressure anomaly by assuming pore-water migration from compacted reservoirs, either arranged in layered formations or represented as swarms of small spheres, toward a dilated zone beneath the décollement. We also compile observations of seafloor crustal deformation driven by SSEs and oceanographic phenomena under baroclinic conditions to refine the spatio-temporal scaling relationship of seafloor pressure variations.

Our main findings are as follows. (i) The potential compacted pore-water reservoirs spatially overlap with the hypocenters of very low-frequency earthquakes (VLFEs), whereas the dilated zone lies in a region with normal-fault-type VLFE activity. (ii) A Kuroshio meander associated with an abrupt fluctuation in sea surface height (SSH) occurred around DONET-1 during the pressure event. (iii) Taken together, (i) and (ii) suggest that the local seafloor pressure change may be explained by pore-water migration destabilized by the Kuroshio current meander. (iv) As this is the first reported case in which a local seafloor pressure anomaly has been identified from only two observation points, the suggested causal link—namely, that the Kuroshio meander may have promoted pore-water migration—provides a strong scientific motivation for future geological surveys, particularly those monitoring seismic activity and seafloor crustal deformation before and after similar pore-water migration events.

How to cite: Ariyoshi, K., Nagano, A., Hasegawa, T., Nakano, M., Matsumoto, H., Aiken, C., Araki, E., Takahashi, N., and Hori, T.: A Local Seafloor Pressure Anomaly Potentially Triggered by Pore Water Migration during Ocean Current Meander, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-271, https://doi.org/10.5194/egusphere-egu26-271, 2026.

EGU26-331 | ECS | Orals | TS1.6

Tracking dehydration reactions and fluid flow in exhuming shear zones using garnet microstructures 

Alessandro Petroccia, Francesco Giuntoli, Alissa Kotowski, Gianmarco Buono, Alireza Chogani, Eric Hellebrand, Lucia Pappalardo, and Ivan Callegari

Shear zones are preferential fluid pathways during prograde and retrograde stages of subduction cycles, but the drainage and permeability of subduction interfaces are poorly quantified. Analyzing exhumed rocks for preserved signatures of fluid production and flow provides insights into fluid circulation during burial and exhumation.

Here, we investigated fluid flow processes recorded by garnets in quartz-schists from the As Sheik shear zone (Saih Hatat window, NE Oman) that records evidence for burial during subduction and local overprinting during exhumation. Garnet occurs as equant, oblate, and honeycomb (i.e., skeletal) shapes, which each documents distinct fluid-related growth stages from peak-pressure to early exhumation associated with a thermal excursion, both occurring at broadly eclogite facies conditions. We show with thermodynamic models and microstructures that garnet first nucleated at 2.0–2.2 GPa and 500–550°C after the chloritoid-out dehydration reaction, which promoted dissolution–precipitation processes. We infer a pseudomorphic replacement of peak-pressure chloritoid by garnet, and based on the absence of internal lattice strain, we suggest that elongate garnet morphology reflects reaction-controlled growth rather than plastic deformation. Our microstructures and models suggest that subsequent decompression and heating (1.5–1.3 GPa, 600–650°C) promoted further fluid release and a renewed stage of honeycomb garnet growth.

We present a conceptual model in which dissolution, transport, and precipitation rates primarily influenced whether garnets grew as oblate grains  (i.e., as pseudomorphs on peak-pressure chloritoid grains), or as newly nucleated equant grains. In addition, we argue that honeycomb garnet represents a snapshot of the permeability network that allowed the fluids to escape from the shear zone using grain boundaries and through reaction-forming pathways.

Using measured maximum mass fraction of fluid released from all the hydrous phases modelled by thermodynamic modelling on a representative rock-scale column of 1000 meters, we estimate the time-integrated fluid flux of the studied shear zone was ~34 m3 m-2 at eclogite facies conditions for the entire duration of garnet growth. This volume represents a limited time-range of the shear zone lifetime during garnet growth, i.e., from peak-pressure to incipient exhumation still at eclogite facies conditions. Therefore, the full lifetime of the shear zone during prograde and retrograde conditions would indeed provide a higher fluid flux.

The different garnet morphologies analyzed all resulted from the chloritoid dehydration reaction, but reflect different rates of dissolution–precipitation and efficiency of dissolution. This study highlights garnet morphology as a tracer of transient fluid pathways during a burial-exhumation cycle of an eclogitic shear zone. The close connection between garnet morphology and fluids calls for a re-evaluation of similar microstructures in different tectonic settings.

How to cite: Petroccia, A., Giuntoli, F., Kotowski, A., Buono, G., Chogani, A., Hellebrand, E., Pappalardo, L., and Callegari, I.: Tracking dehydration reactions and fluid flow in exhuming shear zones using garnet microstructures, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-331, https://doi.org/10.5194/egusphere-egu26-331, 2026.

EGU26-492 | ECS | Posters on site | TS1.6

Towards Absolute dating of Fluid-Flow Remagnetizations: Initial results from Variscan Carbonates 

Catalina Galan, Daniel Pastor-Galán, and Fátima Martín Hernández

Absolute dating of remagnetization events remains the holy grail in paleomagnetism, with the potential to unlock thousands of rock units for new tectonic, metamorphic, and paleointensity studies. Constraining the timing of remagnetizations is especially crucial for understanding fluid flow and mineralogical transformations in orogenic systems.

As a first step toward dating fluid-flow–related remagnetizations, we investigate three Cambrian carbonate units from the northwestern Iberian Peninsula—Tamames, Láncara, and Vegadeo—remagnetized during the Carboniferous. Our goal is to identify, characterize, and ultimately constrain the age of these fluid-induced remagnetization events.

In this presentation we will show an integration of rock magnetism, paleomagnetism, mineralogical, and geochronology results. Magnetic characterization includes room-temperature and low-temperature hysteresis cycles, IRM acquisition curves, First‑Order Reversal Curve diagrams (FORC), thermomagnetic curves, thermal and AF demagnetization, and anisotropy of magnetic susceptibility (AMS). In addition, targeted mineral separation procedures were performed to obtain magnetic sulfide fractions for Re–Os geochronology. The identification and spatial distribution of magnetic phases were examined using scanning electron microscopy (SEM) and quantum diamond microscopy (QDM), allowing us to distinguish primary from secondary magnetic minerals and to evaluate textural evidence of fluid-rock interaction. Complementary U–Pb carbonate geochemistry provides independent age constraints to compare with paleomagnetic and Re–Os datasets.

Together, these results initiate the development of a robust framework for identifying, characterizing, and dating fluid-induced remagnetizations, offering new insights into the tectonic and mineralogical evolution of Iberia’s orogenic systems.

How to cite: Galan, C., Pastor-Galán, D., and Martín Hernández, F.: Towards Absolute dating of Fluid-Flow Remagnetizations: Initial results from Variscan Carbonates, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-492, https://doi.org/10.5194/egusphere-egu26-492, 2026.

White micas breakdown in down-going slabs of subduction zones implies consequent fluids release, inducing element transport into the overlying hanging-wall mantle. Phengite is the most common white mica occurring in HP / UHP metasedimentary rocks, carrying significant amounts of H2O, LILE (K, Ba, Cs and Cr especially), and Li, B or N to the upper mantle. Here,  2H/1H (D/H) and 18O/16O ratios of 23 metapelites samples from the Devonian-Carboniferous Renge and Cretaceous Sambagawa belts are investigated to better understand the O and H isotope signatures of phengites in metapelites of the Pacific-type subduction zone. In addition, we try to constrain the stable isotopic compositions of metamorphic fluids equilibrated with phengites and see their behavior during continuous dehydration reactions.

The investigated pelitic blueschist-facies phengite samples presented non negligeable values of ∂D (∂D < -88‰). 14 of them belong to the Osayama serptentinite melange (central Chugoku Mountains, SW. Japan) of the Renge Belt and separated from lawsonite- and epidotes-grade. They presented a significantly negative ∂D composition, ranging from -113.2‰ to -88.3‰, and a ∂O composition ranging from 12.9‰ to 14.6‰ (∂D and ∂O values approximate SMOW). The 9 other samples are garnet-bearing metapelites of the Sarutagawa schists from Sambagawa Belt (central Shikoku, SW. Japan) and presented ∂D = -95.6‰ to -60.5‰ and ∂O = 12,3‰ to 14,4‰.

Fluids can be characterized as deep-sourced by looking at previous results on high-Si features and K-Ar ages of the investigated samples (Tsujimori & Itaya, 1999). The consequently low values of ∂D cannot be due to meteoric-hydrothermal alteration but by isotopic fractionation during prograde metamorphic dehydration of a plunging slab. Modelling on the obtained data and muscovite, H2O, H and O factors fractionation for nominal temperatures allowed to estimate an isotopic composition for metamorphic fluids equilibrated with phengites. We unveil through this study that slab-devolatilization derived fluids in Pacific-type subduction zone present low ∂D value, implying a non-negligeable role of the phengite breakdown on H isotope composition of nominally anhydrous minerals (NAMs) in deep mantle.

How to cite: Duringer, A., Pastor-Galán, D., Tsujimori, T., Yagi, K., and Álvarez-Valero, A.: Phengite breakdown and associated fluid flow in Pacific-type subduction zone: Investigating the nature of slab-derived fluids of blueschist-facies metapelites from the Renge and Sambagawa belts (SW. Japan)., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-559, https://doi.org/10.5194/egusphere-egu26-559, 2026.

EGU26-964 | ECS | Orals | TS1.6

Fluid-Assisted Deformation: Rhomb Slip Preference in Quartz from Metasomatic Reaction Zones of a Mobile Belt in India 

Subhrajyoti Behera, Anamitra Sikdar, Sumit Chakraborty, and Santanu Misra

Quartz slip systems are conventionally linked with their corresponding temperatures of activation, but fluid can affect them as well; and how the presence of syn-deformational fluid affects the slips system activation remains poorly constrained. Quartz textures are result of integrated effects of P-T-fluid-deformation, making it challenging to isolate the individual contribution of any single factor. The occurrence of metasomatic reaction zones (MRZs) due to fluid-rock interactions at the boundary between country rock, i.e., a pelitic garnet-mica schist and meta-mafic dykes (Dyke-I and -II) in the Northern Singhbhum Mobile Belt (NSMB) of eastern India, provides an opportunity to address this problem. This geometrically well-constrained system, whose P-T-reaction history has been petrologically and geochemically characterized, allows us to isolate and examine how fluids affect the quartz microstructure at same P-T-deformation conditions. We investigated samples from MRZs, using bulk-rock geochemistry, mineral chemistry, thermodynamic modelling and electron backscatter diffraction analysis.

Geochemical-reaction-path models show that MRZs (amphibole-epidote-plagioclase-quartz and chlorite) assemblage formed by Na-metasomatism at 2–3 kbar and 300–500°C after a post-peak condition (6–8.5 kbar and 550–600°C) of NSMB. The saline fluids reacted with the dykes, i.e., the source and then reacted with the pelite, facilitating the element-mass exchange between them. Our study covers two different scenarios, a fluid-abundant MRZs near Dyke-I (zone 1) and another fluid-limited near Dyke-II (zone 2). Zone 1 exhibits a plagioclase-quartz dominated polygonal mosaic matrix with complete removal of muscovite and garnet. The matrix is characterized by pervasive brown-colored anastomosing fluid networks along grain boundaries, fractures, and cleavages. Healed fractures containing Fe-oxide and fluid inclusion trails are abundant, and small epidote grains occur at grain boundaries and triple junctions. Zone 2 is more quartz-dominated with granoblastic texture subhedral grains showing straight to curved boundaries. Relict biotite and garnet are preserved. The matrix quartz shows isolated microfractures and trans-crystal fluid inclusion trails but lacks the extensive interconnected fluid-network architecture of Zone 1.

The slip system of quartz transitions from the country rock towards the two MRZs. Deformation in quartz of the country pelitic schist, was accommodated mainly via activation of prism <a> and <c> slips. They record abundant presence of <2° kernel average misorientation (KAM). Quartz in zone 1 shows deformation accommodation via rhomb <a> slip and near-complete absence of <2° KAM. The intensity of rhomb <a> slip increases towards its dyke-contact. Whereas in zone 2, quartz shows dominant prism <a> slip and abundant <2° KAM, just like the country rock. Near its corresponding dyke contact of zone 2, the quartz shows polygonization, emergence of rhomb <a> slip, and reduction in <2° KAM due to a relatively higher proportion of fluid presence at the contact.

This study demonstrates how fluid-rock-interaction intensity can play significant role in quartz deformations and display a preferred slip system activity under the same prevailing P-T condition. We propose that under fluid-abundant conditions, the quartz polygonised and rhomb <a> slips are activated in zone 1 due to complex reaction creep and hydrolytic weakening resulting from fluid-rock interactions at the same P-T-deformation conditions.

How to cite: Behera, S., Sikdar, A., Chakraborty, S., and Misra, S.: Fluid-Assisted Deformation: Rhomb Slip Preference in Quartz from Metasomatic Reaction Zones of a Mobile Belt in India, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-964, https://doi.org/10.5194/egusphere-egu26-964, 2026.

EGU26-1188 | ECS | Posters on site | TS1.6

Paragenesis of the Munster Basin Upper Devonian polymetallic veins, SW Ireland 

François-Xavier Bonin, Patrick Meere, and Richard Unitt

The Late Paleozoic Munster Basin of SW Ireland is predominantly composed of the non-marine siliciclastic-dominated fine-grained alluvial sediments of the Upper Old Red Sandstone magnafacies. Copper mineralisation in this sedimentary basin is important, either as sediment-hosted stratiform or locally abundant polymetallic vein-hosted copper. In the polymetallic extensional veins, the ore phases include chalcopyrite, tetrahedrite-tennantite, galena, and molybdenite, with gangue minerals commonly quartz, carbonates, chlorite, barite, and Fe-oxides. Recent Re-Os geochronology on molybdenite proved the latter veins opened ca. 367-366 Ma, during Upper Devonian basinal extension, and were deformed before ca. 316-312 Ma by the Variscan orogeny. However, the role of these two major geodynamic events on copper mineralisation was never studied in detail, such that the vein-hosted copper mineralisation and remobilisation processes are still poorly understood. A collection of mineralised vein samples from the western Munster Basin are characterised using reflected light microscopy, Raman spectrometry, and LA-ICPMS trace element analysis to better define the mineralised vein paragenesis. We have identified a pre-mineralisation chlorite veinlet generation. This generation appears to have been reopened by the quartz-rich polymetallic veins in a syntaxial manner, such that the chlorite rims the polymetallic veins. Both vein types show evidence of Variscan deformation (i.e., buckling, displacement). These new observations are critical as 1) the presence of chlorite may allow for precise geothermometry on the veins and 2) the veins appear to have used the same conduits, which may indicate important physicochemical variations (e.g., T, P, pH, fO2, etc.) and/or a pivotal switch in the fluid source(s).

How to cite: Bonin, F.-X., Meere, P., and Unitt, R.: Paragenesis of the Munster Basin Upper Devonian polymetallic veins, SW Ireland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1188, https://doi.org/10.5194/egusphere-egu26-1188, 2026.

The Allihies region on the Beara Peninsula, SW Ireland possesses a mining history for vein-hosted Cu sulphide mineralisation. Structural and chronological control of the deposit has been studied extensively (Fletcher, 1969; Lang et al., 2020; Reilly, 1986; Sheridan, 1964). However, the spatial distribution of fluid alteration in the host rock and associated mineralogy remain unstudied. Several alteration minerals linked with the sulphide mineralisation have been recorded, such as chlorite, muscovite, siderite, calcite, dolomite, kaolinite, montmorillonite, and goethite (Fletcher, 1969).

Reflectance spectroscopy can be used for identifying alteration minerals. Hunt (1977) showed, due to the different electron and molecular structure of the compounds, most minerals absorb unique amounts of energy upon the incident of electromagnetic radiation, thus the reflected energy show characteristics absorption features in the spectra. Certain mineral groups exhibit unique features in the visible-near (400 – 900 nm) and short-wave infrared (900 – 2500 nm) wavelength ranges (Clark et al., 1990; Hunt, 1977). High-spectral resolution (hyperspectral) imaging (HSI) techniques provide a large amount of spectral information where each pixel contains hundreds of narrow, contiguous wavelength bands (Goetz et al., 1985; Lodhi et al., 2019). This gives the ability to identify wavelength positions of mineral absorptions and their subtle deviations that reveal the compositional variations.

Consequently, HSI can be used for analysing the host-rock alterations around the Mountain Mine, Allihies, which will reveal the spatial patterns. The target sulphide mineralisation/lodes are oriented in E-W and N-S (Reilly, 1986), and systematic sampling from the mineralized vein across the alteration zone  will help determine if the fluid alteration has a recognisable detectable spectral signature. Mineral groups such as chlorites, carbonates, and clays (Clark et al., 1990) possibly be differentiated of the existing propylitic and sericitic alteration phases (Fletcher, 1969) as  one moves away from the veins into the country rock.

The current study will use laboratory HS data from a rock scanner for initial analysis, followed by a HS drone survey for extending the spatial scale. Principal Component Analysis will be used for extracting the relevant spectral information (Burger & Gowen, 2011). Subsequently, Minimum wavelength mapper can be incorporated for further analysis of dominating mineral occurrences (Hecker et al., 2019), by studying unique absorption features and their feature depths, for mapping variations across the samples. Specifically, the wavelength range of 2100 - 2400 nm contains the diagnostic absorption features for phyllosilicates and carbonates that highlight the different alteration stages the region has undergone.

The research model has the potential to be further developed for identifying regions with similar spectral responses with mineral exploration potential.

How to cite: Kulugammana, M., Meere, P. A., and Unitt, R. P.: Characterizing the rock alteration associated with vein-hosted Cu sulphide mineralization using hyperspectral reflectance spectroscopy; A case study from the Allihies region, SW Ireland., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1223, https://doi.org/10.5194/egusphere-egu26-1223, 2026.

EGU26-1362 | ECS | Posters on site | TS1.6

Fluid migration, albitization, and metal concentration in the Munster Basin, SW Ireland 

Hannah Vogel, Richard Unitt, and Patrick Meere

Fluids exert a fundamental control on mineral reactions and mass transfer in intracratonic basins, yet the drivers of Na-metasomatism in basins lacking classical evaporite sequences remain poorly understood. The Devonian–Carboniferous Munster Basin of SW Ireland, hosting widespread Cu mineralization, has traditionally been described as containing super-mature arenites with limited feldspar content. However, recent Raman spectroscopic mapping has identified feldspathic sandstones displaying pervasive albitization with at least three different structural varieties of albite providing new insights into a complex history of fluid-rock interaction, and associated metal concentration, across multiple scales.

A detailed petrographic and geochemical analysis is proposed to map the spatial and temporal evolution of albitization in the Munster Basin and investigate how this corresponds with sediment leaching, faulting, and the distribution of metalliferous deposits. To achieve this, three N–S traverses across the basin are conducted, integrating in-situ portable X-ray fluorescence (XRF) measurements to acquire major and trace element data and systematic hand-sampling for laboratory analyses. These basin-scale observations are combined with micro- to nano-scale analytical approaches to investigate (1) the distribution and timing of albitization, (2) the identification of precursor feldspar compositions (K-feldspar vs. plagioclase) through Raman geochemistry, and (3) the implications for sediment leaching and trace-metal mobilization. Portable XRF data are complemented by 2D confocal Raman imaging, petrography, and targeted LA-ICP-MS analysis to constrain fluid chemistry, flow pathways, and the conditions driving feldspar alteration. Particular attention is given to areas adjacent to volcanic centers and major faults, which may have acted as conduits for downward-migrating saline fluids during transgressive events, providing a source capable of inducing pervasive albitization even in the absence of evaporite sequences. 

Preliminary results show systematic variations in albite structural types and associated geochemical signatures that correlate with basin architecture and fault-controlled fluid pathways. By linking grain-scale mineral transformations to basin-scale structural and geochemical frameworks, this study provides new insights into the mechanisms controlling fluid migration, diagenetic alteration, and metalliferous enrichment in post-orogenic intracratonic basins. 

How to cite: Vogel, H., Unitt, R., and Meere, P.: Fluid migration, albitization, and metal concentration in the Munster Basin, SW Ireland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1362, https://doi.org/10.5194/egusphere-egu26-1362, 2026.

The Kettara mining district (Central Jebilet, Morocco) hosts a pyrrhotite-rich massive sulfide lens enclosed within the low-grade metamorphosed Sarhlef volcano-sedimentary sequence and spatially associated with a syntectonic mafic–ultramafic intrusion. The deposit lies within a dextral strike-slip shear zone of the Variscan belt. The main objective of this study is to evaluate the structural role of the Kettara shear zone in the genesis, architecture, and redistribution of the massive sulfide lens, and to determine whether it represents a pre-existing sulfide accumulation subsequently remobilized during ductile deformation or a syntectonic sulfide formation linked to shear-zone activity.

Structural observations reveal an increasing deformation gradient from the volcano-sedimentary wall rocks toward the ore lens, with maximum strain at the ore–host interface. Deformation produced several structural generations: an early S1 foliation with a general N45 orientation associated with anisopachous P1 folds; a penetrative S2 foliation accompanied by tight isoclinal P2 folds; and late chevron P3 folds, observed exclusively within the ore body, which has been tectonically rotated and progressively steepened to a subvertical attitude in direct response to shear-zone deformation. Localized shear corridors exhibit well-developed C/S fabrics, indicating strain partitioning and a strong simple-shear component. These structures acted as preferential pathways for fluid flow, locally accommodating transient porosity through grain-size reduction and recrystallization.

Microscopic studies reveal a mineral paragenesis characterized by two distinct metallogenic stages. The first stage corresponds to a silica- and sulfur-rich fluid, dominated by massive pyrrhotite displaying textures indicative of syn-metamorphic remobilization and recrystallization, accompanied by subordinate pyrite, chalcopyrite, galena, and sphalerite, with chlorite as the main gangue phase. The second stage is characterized by fissuring of pre-existing sulfides and the infiltration of Cu–Zn–Fe-rich fluids, causing disseminated precipitation of pyrrhotite, chalcopyrite, galena, and quartz–carbonates, while reorganizing the minerals under the influence of ductile deformation and the preferential flow of fluids along the structural conduits of the shear zone. Collectively, these stages record the transition from an early Fe-rich massive sulfide accumulation to later fluid-mediated mineral precipitation.

These observations highlight the first-order structural control exerted by the Kettara dextral shear zone on hydrothermal fluid transfer. Although available data do not allow a definitive distinction between metamorphic remobilization of a pre-existing sulfide mineralization and the intervention of magmatic–hydrothermal fluids derived from the syntectonic intrusion, the structural control remains unequivocal. At all scales, the mineralization is strongly guided by the shear-zone architecture, forming anisotropic, high-permeability conduits that control fluid ingress, fluid–rock reactions, and the coupled chemical–mechanical evolution of the deforming rock mass.

Kettara thus represents a natural example of deformation-assisted fluid migration and shear-zone-controlled metallogenesis in an orogenic setting. Complementary petro-structural, geochronological, and isotope geochemistry investigations are needed to constrain the timing, sources, and physico-chemical conditions of the fluids involved.

Keywords: massive sulfides, C/S fabrics, ductile shear zones, fluid flow, remobilization, Kettara.

How to cite: Cisse, D. and Wafik, A.: Deformation-assisted fluid flow and massive sulfide evolution in a ductile shear zone: insights from the Kettara mining district (Central Jebilet, Morocco)., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1754, https://doi.org/10.5194/egusphere-egu26-1754, 2026.

EGU26-1973 | Posters on site | TS1.6

Variation in elemental and Li isotope geochemistry during the weathering of two types of biotite 

Jong-Sik Ryu, Hojin Park, Minjune Yang, and Gi Young Jeong

Lithium (Li) isotopes have been widely used as powerful tracers of chemical weathering processes, providing insights into the coupling between climate and silicate weathering. Although Li isotope fractionation does not occur under equilibrium conditions but rather during kinetically controlled mineral dissolution, the relationship between incipient mineral weathering and Li isotope fractionation remains poorly constrained in natural weathering systems, particularly with respect to the direction and magnitude of fractionation. Here, we investigate elemental and Li isotope geochemistry in two types of biotite—oxidized biotite and hydrobiotite (a 1:1 regularly interstratified biotite–vermiculite)—collected from in situ granitoid weathering profiles. Both biotite types exhibit negative correlations between elemental concentrations and depth; however, Li shows the most pronounced depletion. Elemental loss reaches up to ~70% for Li, with more extensive depletion observed in hydrobiotite compared to oxidized biotite, despite the progressive transformation of biotite into secondary phases such as vermiculite and kaolinite. Lithium isotope analyses are currently underway. By integrating elemental geochemistry with Li isotope compositions, we aim to constrain Li isotope behavior during the initial stages of silicate weathering and to quantify potential Li isotope fractionation associated with distinct biotite alteration pathways. These results will provide new constraints on kinetic controls of Li isotope fractionation during incipient weathering and improve the interpretation of Li isotope signatures in natural weathering systems, including glacial and weathering-limited environments.

How to cite: Ryu, J.-S., Park, H., Yang, M., and Jeong, G. Y.: Variation in elemental and Li isotope geochemistry during the weathering of two types of biotite, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1973, https://doi.org/10.5194/egusphere-egu26-1973, 2026.

Shale oil is predominantly stored in nanoscale pores with ultra-low porosity and permeability, where conventional waterflooding commonly delivers poor recovery. While CO₂-enhanced oil recovery (CO₂-EOR) can improve production by inducing oil swelling, reducing viscosity, and promoting desorption, many existing evaluations still rely on bulk-phase properties and thus inadequately capture nano-confinement and mineral-specific surface effects, obscuring quantitative relationships among CO₂ fraction, desorption efficiency, and mobility. In this study, equilibrium and non-equilibrium molecular dynamics simulations are performed to quantify density layering, competitive adsorption, and rheological/slip behavior of shale oil–CO₂ mixtures confined in quartz and kaolinite nanopores. The simulations show that CO₂ preferentially enriches near pore walls, displaces adsorbed oil, and weakens oil–rock interactions, facilitating the release of interfacial hydrocarbons. Compared with bulk behavior, confinement increases apparent viscosity by about two- to threefold, and kaolinite exhibits pronounced boundary resistance manifested as adverse (negative) slip. As the CO₂ fraction increases to ~20–40%, viscosity decreases markedly and interfacial transport improves, shifting the displacement from unstable fingering toward a more coherent piston-like front. Building on these pore-scale insights, a multiscale coupling framework is developed by embedding MD-derived transport and interfacial parameters into reservoir numerical simulations to conduct 3D field-scale forecasts for the Gulong Sag. The resulting recovery factors that account for nano-confinement (~8–20%) better match field behavior, whereas bulk-parameter simulations substantially overestimate performance. Sensitivity analyses further indicate mineral-dependent economically favorable CO₂ windows (>20% for quartz-dominated pores and ~30–40% for kaolinite-rich pores), highlighting the need for differentiated injection strategies; overall, the proposed multiscale approach bridges microscopic interfacial physics and macroscopic development prediction, providing quantitative support for optimizing CO₂-EOR and enhancing CO₂ utilization and storage in unconventional reservoirs.

Keywords: Shale oil; Nano-confinement effects; Molecular dynamics simulations; Unconventional reservoirs

How to cite: Liu, H. and Xue, H.: Effect of CO2 Pre-Extraction on Water Flooding in Nanopores: Insights from Molecular Dynamics Simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2439, https://doi.org/10.5194/egusphere-egu26-2439, 2026.

EGU26-3448 | Posters on site | TS1.6

Interplay Between Migmatites and Deep Crustal Shear Zones 

Bruna B. Carvalho and Edward W. Sawyer

The presence of melt and associated fluids profoundly weakens the continental crust, promoting strain localization and establishing a close link between migmatites and ductile shear zones. Here we compare four migmatite case studies developed within major crustal-scale shear zones formed in contrasting tectonic settings, from collisional to extensional regimes: the Kinawa migmatite (Brazil), Opatica migmatite (Canada), Saint-Malo migmatite (France), and the Øksfjord Shear Zone (Norway). Our goal is to evaluate the connection between migmatites and shear zones, their impact on shear zone evolution, and the main macro- and microstructural features of migmatites in shear zones. We also examine the extent to which shear zones may serve as conduits for magma transport within the crust.

All migmatites formed at mid- to lower-crustal conditions (4–9 kbar; 650–820 °C) under both fluid-present and fluid-absent regimes. Macro- and microstructural observations reveal that the evolution of melt connectivity and permeability was strongly controlled by shear zone kinematics. In the Kinawa and Opatica examples, preservation of magmatic microstructures indicates that deformation ceased shortly after melt crystallization, suggesting limited post-melting deformation. In contrast, the Saint-Malo and Øksfjord shear zones record pervasive solid-state deformation overprinting magmatic fabrics, implying sustained deformation and continued microstructural reorganization after partial melting.

Across all examples, the spatial association between migmatites and shear zones highlights the role of deformation in enhancing melt segregation, extraction, and transient permeability. However, only some shear zones evolved into efficient pathways for melt migration. These and other case studies from the literature illustrate how ductile shear zones function as dynamic crustal domains in which deformation, partial melting, and fluid transport are tightly coupled, and where porosity and permeability evolve through time in response to changing rheology and strain.

How to cite: Carvalho, B. B. and Sawyer, E. W.: Interplay Between Migmatites and Deep Crustal Shear Zones, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3448, https://doi.org/10.5194/egusphere-egu26-3448, 2026.

Fluid-rock interactions drive critical lithospheric processes and industrial applications including CO₂ storage and geothermal energy extraction. In deep crystalline crust where static permeability is negligible and rocks do not deform, fluids primarily exploit transient pathways created through chemical reactions with minerals in disequilibrium. These reaction-induced pore networks dynamically alter rock permeability, yet their ephemeral nature makes direct characterization challenging.

We present an integrated methodology combining time-resolved synchrotron x-ray microtomographic imaging (4DSµCT) with generative artificial intelligence to quantify reaction-induced porosity evolution. Using 4DSµCT, we captured spatio-temporal pore network dynamics during KBr-KCl replacement, a well-established analogue for interface-coupled dissolution-precipitation processes. Advanced statistical microstructural descriptors and Minkowski functionals revealed intricate coupling between dissolution-precipitation mechanisms, transport regimes, and evolving connectivity governing transient permeability.

To extend insights beyond experimental limitations, particularly for high-temperature systems (>500°C) where direct imaging remains infeasible, we developed Pore-Edit GAN, a StyleGAN2-ADA framework trained on ~29,000 tomographic images. This model generates statistically realistic microstructures while enabling semantic editing of porosity and connectivity. We applied our approach to hydrothermally altered monzonite from the Oslo Rift, where feldspar replacement reactions at ~10 km depth created now-isolated pore networks. By navigating the GAN latent space along learned connectivity directions, we reconstructed plausible transient pore configurations, effectively reversing the porosity isolation that occurred as reactions ceased.

Voxel-based finite element simulations of incompressible Stokes flow through these AI-reconstructed networks yield permeabilities reaching 4.5×10⁻¹⁵ m², a two-order-of-magnitude enhancement upon pore reconnection, consistent with established transient crustal permeability-depth relations. This convergence of synchrotron capabilities, deep generative models, and computational fluid dynamics establishes a quantitative framework for predicting transport properties in reactive geological systems where direct observation remains challenging.

How to cite: Plümper, O., Amiri, H., and Fusseis, F.: Reaction-Induced Porosity During Fluid-Mineral Interaction: From 4D Synchrotron Imaging to AI-Driven Permeability Reconstruction, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3949, https://doi.org/10.5194/egusphere-egu26-3949, 2026.

Fluid flow through ductile shear zones is increasingly recognised as a key control on the localisation, upgrading, and redistribution of hydrothermal ore systems. We investigate how syn-deformational porosity evolves with increasing finite strain in a calcite-rich marble mylonite from the Western Mary Kathleen shear zone adjacent to the Mary Kathleen REE-U deposit (NW Queensland, Australia). Microstructural evolution and pore-network topology are tracked along a natural strain gradient using electron backscatter diffraction (EBSD) and synchrotron micro-computed tomography (3-D micro-CT). EBSD reveals a progressive transition from twin-rich, dislocation-dominated calcite fabrics at lower strain to uniformly fine-grained, foam-like mosaics at higher strain, where grain-size-sensitive deformation (diffusion creep and grain-boundary sliding) dominates and crystallographic preferred orientations weaken. In lower-strain mylonites, pores occur mainly as isolated to weakly connected cavities along subgrain and grain boundaries, concentrated at boundary junctions and locally associated with twin lamellae. With increasing strain and grain-size reduction, porosity reorganises into fewer but larger, high-aspect-ratio grain-boundary networks that link into laterally continuous pore sheets. Micro-CT-derived orientations show that the normals to these sheets cluster near the instantaneous shortening direction, indicating that connected pore sheets are commonly oblique to both the S- and C-planes rather than strictly foliation-parallel. These results demonstrate that finite-strain-driven grain-size reduction can generate transient, strongly anisotropic permeability by organising boundary-hosted porosity into interconnected, sheet-like conduits, providing a plausible microstructural mechanism for deformation-controlled fluid focusing and REE-U-bearing fluid redistribution in carbonate shear zones.

How to cite: Olesch-Byrne, A., Finch, M., and Vieira Ribeiro, B.: The evolution of syn-deformational porosity in a marble mylonite over increasing strain: Insights from EBSD and 3-D microcomputed tomography, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4662, https://doi.org/10.5194/egusphere-egu26-4662, 2026.

EGU26-6268 | ECS | Posters on site | TS1.6

Acoustic Characterization of Fluid Seepage Controlled by Tectonic Structures Offshore Southwestern Taiwan 

Cheng-Yu Ou, Tzu-Ting Chen, Ho-Han Hsu, and Yen-Chi Wu

This study quantifies spatial variations in acoustic seepage intensity offshore southwestern Taiwan and assesses whether margin setting or conduit continuity better explains the observed differences. Seepage variability was characterized using volume backscattering strength (Sv), plume geometry, and subsurface structural features. A total of 21 plumes from 14 seep sites were characterized based on Sv and geometry derived from Simrad EK60/EK80 echosounder data. After applying transmission-loss correction, seepage sites on the passive margin (e.g., Horseshoe Ridge, Pointer Ridge, and Formosa Ridge) exhibit higher Sv and taller plumes than those on the active margin. Integration with multichannel seismic profiles and sediment-core records reveals extensive free gas beneath bottom-simulating reflectors (BSRs) and gas chimneys, indicating sustained fluid migration through persistent conduits. In contrast, relatively weak Sv at the mixed-origin G96 site suggests partial conduit infilling. These observations indicate that although tectonic deformation establishes the first-order structural framework for fluid migration, the continuity and evolutionary state of seep conduits exert the dominant control on seepage intensity. Potential tidal modulation was further evaluated by comparing Sv with the rate of tidal pressure change, but only weak correlations were observed, suggesting that tidal forcing plays a secondary role in controlling seepage variability.

Keywords: seepage intensity, margin setting, conduit continuity, volume backscattering strength (Sv), offshore southwestern Taiwan

How to cite: Ou, C.-Y., Chen, T.-T., Hsu, H.-H., and Wu, Y.-C.: Acoustic Characterization of Fluid Seepage Controlled by Tectonic Structures Offshore Southwestern Taiwan, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6268, https://doi.org/10.5194/egusphere-egu26-6268, 2026.

The Upper Rhine Graben (URG) is the central part of the European Cenozoic Rift System and holds a huge geothermal potential due to a reduced Moho depth and active hot brine convection cells. In addition to that appealing potential, hydrothermal brines of the URG show high Lithium concentrations. Yet, investors-relying deep geothermal energy companies face difficulties to predict fracture network permeability before drilling operations. This problem induces techno-economic risks, which frighten investments and in turn hinder the wide development of deep geothermal energy use. The goal of this work is to provide input data to develop modelling tools to help predict fracture network permeability before drilling operations. We will integrate data from both the French and German side of the URG, which is seldomly done in studies. Here we present a timeline that we’ll use as a data compilation base to reconstruct the URG setup and hydrothermal fracture clogging history. Once identified, the fracture clogging events will be deeper characterized to be implemented in a reconstruction model. A characterization of mineralized fractures all around the URG shoulders will help to complete the list of hydrothermal clogging events identified in the Black Forest (Permian, Jurassic-Cretaceous and Paleogene) and will allow to simulate the rate of precipitation in mineralized fractures and thus their clogging potential.

How to cite: Mazzinghi, L.: A timeline for the reconstruction of Upper Rhine Graben hydrothermal fracture mineralization events  , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7761, https://doi.org/10.5194/egusphere-egu26-7761, 2026.

EGU26-7824 | Posters on site | TS1.6

Geological process understanding in space and time 

Daniel Koehn and Sandra Piazolo

Geological patterns in space and time are dependent on a number of processes that scale differently depending on whether or not they are linear or non-linear and on the involved constants (rate constants, diffusion constants). In order to predict geological processes and their occurrence in space and time one needs to understand at what spatio-temporal scales they are active. Quite often the slowest process is dominating the time scale of pattern evolution, therefore cross-over points in space and time are of special interest, where the dominance of one processes over another switches. When two processes are competing during the formation of a pattern, the cross-overs are critical points where the behavior of the system changes. Here we are exploring five important processes namely elastic wave propagation, fluid pressure diffusion, temperature diffusion, matter diffusion and reactions. While elastic wave propagation and reactions scale linearly, fluid pressure-, temperature-, and matter-diffusion have non-linear scaling behavior, which can be illustrated best in a log-log diagram of time versus space. In such a diagram the diffusion processes have a steeper slope than the two linear processes. Fluid pressure diffusion is 3 to 4 orders of magnitude faster than temperature diffusion, which itself is 3 orders of magnitude faster than matter diffusion (in a fluid). For example if a reactive fluid enters a fault, in a second the fluid pressure equilibrates on a m-scale, the temperature on a mm-scale and matter on the micro-meter scale. During fault slip that happens due to fluid overpressure, elastic wave propagation and fluid pressure diffusion act at the same time scale on micrometers but then diverge with fluid pressure diffusion equilibrating in seconds on the m-scale while elastic wave propagation reaches km-scale at the same time. We will discuss these scaling relations in details with examples from a variety of geological processes.

 

How to cite: Koehn, D. and Piazolo, S.: Geological process understanding in space and time, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7824, https://doi.org/10.5194/egusphere-egu26-7824, 2026.

EGU26-8033 | ECS | Posters on site | TS1.6

Wrinkled clocks in the crust: dating deformation in Archean gold-bearing shear zones 

Isabelle Komendat, David Schneider, and Renelle Dubosq

Mid-crustal shear zones localize strain and control the migration of heat and fluids, making them central to understanding metallic ore-forming processes. Mica are widely used to date deformation in shear zones, however their radiometric ages can be difficult to interpret because hydrothermal alteration and strain-induced microstructural defects can promote recrystallization and disrupt isotopic retention. In Archean gold camps, mica ages commonly postdate mineralization events by >100 Myr, raising questions about whether these ages reflect primary mineralization, metamorphic or hydrothermal growth, or post-orogenic remobilization. Robust interpretation of these ages requires direct integration of geochemical and micro- to nanoscale structural analysis. We examined mica from the Sunday Lake Deformation Zone, a regional scale deformation zone controlling gold mineralization at Agnico Eagle Mines Ltd. giant Detour Lake Mine (DLM), in the northwestern Abitibi greenstone belt, Canada. The DLM orogenic gold deposit is characterized by c. 2734-2724 Ma volcanic rocks, comprising ultramafic-dominated lower units and mafic volcanic and volcaniclastic upper units, metamorphosed under greenschist to lower amphibolite facies conditions. Mafic host rocks are intruded by felsic to mafic sills and dikes. The main regional foliation is subvertical and axial-planar to west-trending, shallowly-plunging tight to isoclinal folds, which transposes the intrusive relationships. Gold mineralization occurred at c. 2670-2640 Ma in a syn-orogenic setting. Microstructural analyses were conducted on muscovite from felsic meta-intrusive rocks, collected from drill core, that are comprised of quartz, muscovite ± biotite, plagioclase, K-feldspar, chlorite, garnet, amphibole, carbonates and sulfides. Quartz microstructures record bulging recrystallization and nascent subgrain rotation, indicating deformation temperatures of ~300-400°C. Plagioclase display tapered deformation twins and brittle fracturing, consistent with low to moderate temperature deformation. Mica constitute between <5 and 30 vol% of the rock and occur as euhedral porphyroblasts/neoblasts to subhedral poikilitic, skeletal grains ranging in size from 15 x 50 μm to 250 x 650 μm. High-resolution electron channeling contrast imaging of the mica reveals weak undulatory orientation contrast patterns perpendicular to cleavage planes in ~20-50% of the grains. Such contrast patterns suggest deformation in the mica is accommodated primarily by dislocation glide. Backscatter electron imaging of the mica also revealed concentric chemical zoning, typically expressed as irregular and discontinuous rims along grain margins, which are weakly enriched in Fe and Al and depleted in Mg and Si relative to mica cores. Muscovite Ar-Ar analyses from unmineralized rocks at DLM yield single-crystal dates of 2600-2100 Ma, and complementary K-Ca and Rb-Sr dating will be conducted to assess the roles of Ar loss and element mobility in producing these younger and dispersed ages. The timing of metamorphism and deformation has important implications for understanding the nature and controls on mineralization at DLM, and whether the original geometry and mineralogy of the deposit has been modified through later stages of syn‐metamorphic deformation.

How to cite: Komendat, I., Schneider, D., and Dubosq, R.: Wrinkled clocks in the crust: dating deformation in Archean gold-bearing shear zones, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8033, https://doi.org/10.5194/egusphere-egu26-8033, 2026.

EGU26-8377 | ECS | Posters on site | TS1.6

Carbon gradients as tracers of structurally controlled fluid flow in homogeneous metabasaltic sills (Loch Stornoway, Scottish Highlands). 

Yessica González-Ixta, Barbara Kleine-Marshall, Alasdair Skelton, and Daniel Koehn

In the past decades, the extent of fluid-induced reaction halos in metabasaltic sills within the Argyll Group of the Dalradian Supergroup in the SW Scottish Highlands has been intensively used to constrain metamorphic fluid flow velocities (Skelton, 2011). However, recent findings revealed that reaction front propagation within numerous sills was primarily controlled by preferred fabric alignment at the margins during deformation events, as well as by mineralogical and chemical heterogeneities across the sills. Here, we revisit hydration and carbonation fronts in metabasaltic sills in the vicinity of major fluid pathways, i.e., the Loch Awe Syncline and Ardrishaig Anticline, to reevaluate fluid-induced reaction front propagation and constrain metamorphic fluid flow velocities.
This study integrates field observations, detailed petrological-textural analyses, and whole-rock geochemistry, including carbon and water contents as well as trace element data, along a transect across compositionally homogeneous metabasaltic sills. The aim is to constrain the mechanisms controlling fluid-induced reaction progress at the contact between metasedimentary rocks and metabasaltic sills.
The selected basaltic sills were metamorphosed under greenschist- and epidote-amphibolite-facies conditions and record at least four deformation events. In the sill margins, the rocks show increased calcite and chlorite contents and replacement of garnet, amphibole, and dark mica, reflecting localized retrogression. This retrograde overprint is also characterized by mobilization of large-ion lithophile elements (LILE; e.g., K, Na, Sr). In contrast, the sill interior preserves textural and mineralogical equilibrium among amphibole, dark mica, epidote, garnet, and titanite. Textural variations indicate a progressive decrease in hydration and carbonation toward the sill interior.
Carbon contents decrease systematically from 1.22-1.16 wt.% in the sill margins to 0.07-0.02 wt.% toward the sill interior. Similarly, water contents are highest in the sill margins (up to 1.95 wt.%) and lowest in the sill interior (0.52 wt.%). Petrographic observations further suggest that fluid infiltration and reaction are controlled by structural anisotropy inherited from earlier deformation during retrogression, rather than mineralogical heterogeneity. Fluid flow is preferentially channelized along lithological contacts and deformation-related weaknesses, such as foliation and mineral lineation, which are most developed near the sill margins.
The new dataset enables a recalculation of the true spatial extent of metamorphic fluid infiltration and allows time-integrated estimates of fluid fluxes based on carbonation and hydration reaction front geometries, as well as their relationships with trace element redistribution. Understanding the rates of CO₂ release and sequestration during orogenic processes provides new insights into the role of structural anisotropies and brittle-ductile processes in controlling the volume, pathways, and metal-enriching potential of metamorphic fluid flow.

How to cite: González-Ixta, Y., Kleine-Marshall, B., Skelton, A., and Koehn, D.: Carbon gradients as tracers of structurally controlled fluid flow in homogeneous metabasaltic sills (Loch Stornoway, Scottish Highlands)., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8377, https://doi.org/10.5194/egusphere-egu26-8377, 2026.

EGU26-9560 | ECS | Posters on site | TS1.6

Strike-slip fault system and fluorite mineralization in the Hongjianbing area, Mazong Mountain, Gansu China 

Chao Bo, Genhou Wang, Peilie Zhang, and Jingqi Zhang

Abstract: The Beishan Orogenic Belt, located along the southern margin of the Central Asian Orogenic Belt, is one of the key mineral resource regions in northwestern China. The Hongjianbing fluorite deposit, located in the northern part of this belt, is a well-known quartz-vein-type fluorite deposit that has attracted considerable attention from researchers. Through field geological mapping, UAV and remote sensing measurements, and borehole structural recording, two east–west-trending strike-slip fault systems were identified in the study area, separated by a distance of 5 km, with nearly vertical dips. These faults exhibit multi-stage activity, with early deformation characterized by dextral strike-slip motion. The intervening blocks experienced ductile deformation, with S-C fabric development in the shear zones.39Ar-40Ar dating of biotite from the mylonite in the ductile shear zone yielded a plateau age of approximately 330 Ma, marking the timing of ductile deformation. Later, these two faults evolved into brittle left-lateral strike-slip faults, forming a Riedel shear system (R, R', T shears), and displaying fault breccia and fault gouge. K–Ar dating of authigenic illite from the fault gouge yielded an age of approximately 220 Ma, indicating a transition from ductile to brittle deformation over time.The host rocks of the fluorite deposit are mainly intermediate to acidic volcanic rocks from the Carboniferous Baishan Formation. Zircon U–Pb dating of these rocks yielded ages of approximately 330 Ma, suggesting that the host rocks may have formed during contemporaneous magmatic activity. All fluorite orebodies are located within the main damage zone of the southern brittle fault system, which exhibits left-lateral, right-stepping characteristics. The development of this brittle fault system provided the necessary space and conduits for ore-forming fluid migration, facilitating fluorite mineralization.The cataclastic texture of the ores further suggests that mineralization occurred after significant faulting, reflecting high fluid mobility within the fault damage zones. This high fluid mobility is also reflected in the characteristics of the fluorite ore bodies. After migrating along the brittle fault zones, mineralizing fluids precipitated fluorite as fine veinlets, which is the current form of mineralization observed in the deposit. A three-dimensional geological model of the ore body was constructed using GOCAD software, revealing the close temporal and spatial relationship between fluorite mineralization and fault activity.
Keywords: Structural control of mineralization; Fluorite deposit; Geochronology; Three-dimensional mineralization model;

How to cite: Bo, C., Wang, G., Zhang, P., and Zhang, J.: Strike-slip fault system and fluorite mineralization in the Hongjianbing area, Mazong Mountain, Gansu China, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9560, https://doi.org/10.5194/egusphere-egu26-9560, 2026.

EGU26-10973 | ECS | Orals | TS1.6

Fluid–rock interactions in a crustal-scale upflow system: syn-rift albitization of the North-Pyrenean Massifs 

Camille Jansen, Yoann Denèle, Guillaume Estrade, Oscar Laurent, Mathieu Leisen, and Michel de Saint-Blanquat

Understanding how solid-state deformation and fluid flow interact is essential to constrain continental lithosphere evolution. The North-Pyrenean Zone, located in the Pyrenean retro-wedge, corresponds to an inverted Early Cretaceous rift that led to mantle exhumation. It comprises Mesozoic basins and Variscan basement massifs. Key rifting markers include: (i) thick Albian-Cenomanian detrital sequences, (ii) peridotite bodies reworked into pre-/syn-rift sediments, (iii) HT–LP metamorphic paragenesis in pre-/syn-rift series, and (iv) giant metasomatic stocks comprising talcschist and albitite. Although geochronological data show that metasomatic bodies are related to large-scale fluid circulation during Early Cretaceous rifting (130–90 Ma), the associated 3D–4D fluid circulation system remains poorly constrained.

Our study focuses on the eastern part of the Arize North-Pyrenean Massif, a syn-rift tilted block exposing, beneath a pre- and syn-rift halokinetic sedimentary cover, a complete Variscan metamorphic series from migmatites to the South, to low-grade Carboniferous pelites to the North. While foliation trajectories are homogeneously N100°-oriented across the western and central parts of the Arize massif, its eastern part is distinguished by a heterogeneous foliation pattern within a N140°E-oriented, transtensional folded and faulted zone. A pervasive metasomatic zone is developed within a 10 km² elliptical domain at the core of this structural system. It encompasses pure albitite stocks and results from a two-stage alteration process. The least metasomatized samples show minor plagioclase alteration and biotite destabilization, with newly crystallized titanite, apatite and epidote. Whole-rock data reveal a strong Ca-enrichment mainly hosted in the newly formed Ca-rich mineral assemblages. The most metasomatized samples exhibit quartz leaching and albitization of plagioclase associated to relatively limited net chemical change. Fluid inclusions trapped in metasomatized apatite contain H2O–NaCl–CaCl2 brines (≈ 16 wt.% NaCl eq.), recording trapping conditions of ~300 °C and ~205 MPa. Quartz generally shows no evidence of crystal-plastic deformation, despite its plasticity temperature being close to the inferred fluid trapping temperatures. Locally, a structural transition, marked by late low-angle normal faults associated with C-S structures and, in places, mylonites, documents increasing system temperature. This thermal increase is interpreted as resulting from progressive heating of the surrounding rocks by circulating fluids.

We interpret the Arize fossile hydrothermal fluid system as a transient reservoir of ascending hot fluids located above a transient brittle–ductile transition. In such a system, downwelling fluids are stored at the brittle–ductile transition, where subhorizontal anisotropy planes act as impermeable barriers. Locally, these fluids, heated to 300–400 °C, ascend into the upper crust along vertical anisotropy planes (tilted Variscan foliations) and brittle structures (faults). U–Pb dating of newly formed titanites at ca. 130 Ma supports the interpretation that metasomatism in the Arize upflow system occurred during the early stages of rifting. Finally, we demonstrate that, at the scale of the Pyrenean rift, the Arize hydrothermal system, located within an oblique transtensional zone, developed in a syn-rift linkage zone between N100°E-oriented rift segments. This integrated study underscores the role of fluid flow in linkage zones associated with continental crust stretching, with implications for hydrothermal and geothermal systems.

How to cite: Jansen, C., Denèle, Y., Estrade, G., Laurent, O., Leisen, M., and de Saint-Blanquat, M.: Fluid–rock interactions in a crustal-scale upflow system: syn-rift albitization of the North-Pyrenean Massifs, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10973, https://doi.org/10.5194/egusphere-egu26-10973, 2026.

EGU26-11377 | ECS | Posters on site | TS1.6

Fluid flow in foreland basins: spatial and temporal scaling of their transport mechanisms 

Lisa Lebrun, Barbara Kleine-Marshall, and Daniel Koehn

Foreland basins often host important ore deposits (like MVT deposits; Bradley and Leach, 2003) which are associated with deep and shallow fluid circulation. Those fluids, expelled from the orogen, can have different origins like meteoric water, diagenetic fluid, metamorphic fluid or even deeper crustal origins (Oliver J., 1986). However, whether these fluids are expelled to the foreland as continuous flow or as series of rapid pulses remains largely unexplored. Here, we combine numerical modelling with geochemical data and petrographic observation of a sandstone and its associated veins and reaction halos to identify spatial and temporal fluid flow and its transport mechanism(s) in foreland basins.

Thin sections from a Rotliegend red arkose-sandstone formation (German Permian Variscan foreland) were investigated using microprobe analysis and BSE-EDS-SEM imaging. The arkose-sandstone exhibited tapering lighter reaction halos around veinlets, most likely produced through redox reactions upon fluid infiltration into the sandstone. The model Elle from Koehn et al., (2022) was subsequently applied to link fluid transport mechanism to the patterns and geometry observed in the samples. Pore pressure applied from a crack toward the host rock and a concentration gradient were used to create fluid flow in the sandstone from which a range of values for advection, diffusion and a reaction rate were deduced. In this way, the model allowed to mimic the same pattern/geometry as the sample on several scales and enabled a systematic assessment whether fluid flow may have been constant or pulsating.

Combining petrographic, geochemical and modelling investigations revealed that the reaction halos in the sandstone were in fact formed upon a single rapid fluid flow event, that presumably was fast and channelised in the vein, and pervasive and comparatively slow in the surrounding host rock. These preliminary results imply that fluid flow and transport in foreland basins may be of a more pulsating nature rather than continuous steady state fluid flow and transport mechanisms may thus be similar to what has been previously reported for subduction zone settings (e.g., Kleine et al., 2016).

Bradley, D. C., & Leach, D. L. (2003). Tectonic controls of Mississippi Valley-type lead–zinc mineralization in orogenic forelands. Mineralium deposita38(6), 652-667.

Kleine, B. I., Zhao, Z., & Skelton, A. D. (2016). Rapid fluid flow along fractures at greenschist facies conditions on Syros, Greece. American Journal of Science316(2), 169-201.

Koehn, D., Kelka, U., Toussaint, R., Siegel, C., Mullen, G., Boyce, A., & Piazolo, S. (2022). Outcrop scale mixing enhanced by permeability variations: the role of stationary and travelling waves of high saturation indices. Geological Magazine159(11-12), 2279-2292.

Oliver, J. (1986). Fluids expelled tectonically from orogenic belts: their role in hydrocarbon migration and other geologic phenomena. Geology14(2), 99-102.

How to cite: Lebrun, L., Kleine-Marshall, B., and Koehn, D.: Fluid flow in foreland basins: spatial and temporal scaling of their transport mechanisms, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11377, https://doi.org/10.5194/egusphere-egu26-11377, 2026.

EGU26-11563 | Posters on site | TS1.6

Hydro-Mechanical Modeling of Over-Pressured Mobile Shale: Insights into Shear Dilation Effects on the Uplift at Zhong Liao Tunnel, Taiwan 

Eh Tan, Chia-Hsun Lin, Wei-Hau Wang, Maryline Le Beon, and Taras Gerya

Mobile shales strongly influence deformation, uplift, and fluid migration in compressional sedimentary basins, yet the mechanical pathway from "normal" shale to mobile shale is still debated. This study tests the idea that shear-induced dilation under high pore-fluid overpressure can trigger a positive feedback among shear localization, porosity–permeability increase, and fluid flow, thereby promoting long-lived, ductile-like shale mobility. We focus on the Zhongliao Tunnel area in southwestern Taiwan, where rapid uplift and sharp spatial gradients in vertical motion have been reported near major faults.

We develop a two-phase hydro-mechanical numerical model that couples a poro–visco–elasto–plastic solid with Darcy fluid flow. Porosity evolves through competing compaction and a strain-rate–dependent dilation term that is activated under elevated overpressure, allowing fault-related shear zones to dynamically transform into high-permeability conduits. In the reference experiment, a high-pressure layer sealed beneath a low-permeability cap sustains overpressure within mudstone. Once shear localizes, dilation increases porosity and permeability along damage zones, enhancing focused fluid discharge. The resulting seepage forces and reduced effective strength further intensify shear localization, producing sustained fault creep and pronounced uplift of the block bounded by the principal fault systems. The modeled uplift pattern reproduces key first-order observations: a sharp vertical-velocity contrast across the main fault and a more gradual decay of uplift away from it, with peak uplift rates reaching the order of centimeters per year.

Sensitivity tests demonstrate that overpressure alone generates only modest uplift without dilation-enabled conduit formation, while shear compaction suppresses localization and distributes deformation. Permeability exerts a non-monotonic control: very low permeability limits fluid flux and seepage forcing, whereas very high permeability drains overpressure too efficiently and weakens sustained creep. Overall, the results provide a mechanistic framework for how overpressured mudstone can evolve into mobile shale through coupled dilation and fluid flow, and offer testable criteria for identifying similar processes in other shale-dominated orogenic settings.

How to cite: Tan, E., Lin, C.-H., Wang, W.-H., Le Beon, M., and Gerya, T.: Hydro-Mechanical Modeling of Over-Pressured Mobile Shale: Insights into Shear Dilation Effects on the Uplift at Zhong Liao Tunnel, Taiwan, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11563, https://doi.org/10.5194/egusphere-egu26-11563, 2026.

EGU26-12850 | ECS | Orals | TS1.6

A multi-scale hierarchical FEM-DEM approach for hydro-chemo-mechanical modeling of granular media 

Ehsan Ahmadi Olyaei and Daniel Koehn

Numerical study of phenomena in granular media is typically classified into two categories according to the scale of the domain: macro-scale modeling which relies primarily on continuum theories, such as the Finite Element Method (FEM), and micro-scale modeling, which is based on interparticle forces, commonly performed using the Discrete Element Method (DEM).

However, granular/porous media are inherently discontinuous due to their micro-structure, and traditional continuum-based approaches cannot accurately capture microstructure-induced anisotropy in these media. Particle-based approaches like DEM have therefore been widely used for the modeling of such discontinuous domains.

On the other hand, it is not computationally feasible to resolve the entire intricate microstructure of large domains using DEM. Thus, this work implements a multi-scale approach that combines the accuracy of DEM at the grain scale with the computational efficiency of FEM at the macro-scale.

The approach is called “Hierarchical FEM-DEM”, originally developed to study the mechanical response and strain localization (shear bands) in granular media [1]. It then has been extended to hydro-mechanical problems in saturated media [2]. In this framework DEM assemblies are treated as Representative Volume Elements (RVE) attached to Gauss (integration) points of a macroscopic FEM mesh. The DEM is used for the calculation of the homogenized effective stress corresponding to the interpolated strain field on each Gauss point, thereby eliminating the need for phenomenological constitutive assumptions for the solid skeleton, that are common in conventional nonlinear FEM analyses.

In this study we apply this method by implementing it in MATLAB to investigate the hydro-chemo-mechanics of granular media. The model is going to be used to study the effect of fluid flow and pore pressure on the solid skeleton deformation, and generation of shear bands, how micro-scale solute-related heterogeneities influence the macro-scale mechanical behavior, based on thin sections made from field sample collected by the authors.

We use periodic boundary conditions for DEM assemblies to satisfy the compatibility between the microscopic deformation and the macroscopic strain field imposed at the Gauss points, ensuring the condition for the satisfaction of Hill-Mandel micro-macro energy equivalence during homogenization. At the macroscopic level, the boundary conditions are prescribed to simulate the in-situ loading and hydraulic conditions, corresponding to the field sites from which the samples were extracted.

References

[1] Guo, N. and Zhao, J., 2014. A coupled FEM/DEM approach for hierarchical multiscale modelling of granular media. International Journal for Numerical Methods in Engineering99(11), pp.789-818.

[2] Guo, N. and Zhao, J., 2016. Parallel hierarchical multiscale modelling of hydro-mechanical problems for saturated granular soils. Computer Methods in Applied Mechanics and Engineering305, pp.37-61.

How to cite: Ahmadi Olyaei, E. and Koehn, D.: A multi-scale hierarchical FEM-DEM approach for hydro-chemo-mechanical modeling of granular media, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12850, https://doi.org/10.5194/egusphere-egu26-12850, 2026.

The particle migration phenomenon in porous media exhibits dual effects: it can both impede fluid flow and regulate the flow field. The temporary plugging effect induced by particle migration can delay the formation of preferential flow paths in waterflooding and enhance recovery efficiency. However, research on actively controlling the flow field through particle migration to improve recovery efficiency is still limited. This study aims to investigate the generation of a temporary plugging effect within the pores by controlling the particle size and concentration in the injected water, thereby regulating the distribution of the flow field and enhancing oil recovery. The research combines numerical simulation techniques with core flooding experiments, constructing numerical models with different micro-pore structure characteristics, such as moldic pores and intrafossil pores, and physical models with varying permeability gradients. Experimental results show that after the formation of preferential flow paths in waterflooding, continued water injection can no longer effectively displace the remaining oil in the porous media. At this point, the addition of suspended particles (median particle size: 5 μm, concentration: 200 mg L⁻¹) to the injected water further enhances displacement. The particles migrate with the water flow and preferentially accumulate in high-connectivity pores and throats, forming a temporary plugging effect. This alters the local flow path, expanding the sweep volume of waterflooding and effectively mobilizing oil in low-permeability pores.

When the particle size exceeds 10 μm or the concentration exceeds 400 mg L⁻¹, bridging or sealing effects are likely to occur at pore entrances, severely obstructing fluid flow. Conversely, when the particle size is too small (<2 μm) or the concentration too low (<10 mg L⁻¹), the particles fail to effectively retain and do not form a significant temporary plugging effect. After the particle-based flow regulation treatment, the final oil recovery efficiency of the model can be increased by approximately 10% to 20%.

How to cite: Penglei, Y.: Regulation of Fluid Flow Behavior in Porous Media Based on Particle Migration, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13057, https://doi.org/10.5194/egusphere-egu26-13057, 2026.

EGU26-14061 | Posters on site | TS1.6

Stylolite-controlled dolomitization and dedolomitization in low-porosity carbonates (Lessini Mountains, Southern Alps, Italy) 

Costantino Zuccari, Gianluca Vignaroli, Fabrizio Balsamo, Luigi Berio, Gianmarco Buono, Lucia Pappalardo, and Giulio Viola

Dolomitization is among the most widespread processes affecting carbonate rocks and may significantly overprint carbonate successions during post-diagenetic and deformation-related fluid infilling and circulation. The process is generally hindered in low-porosity/low-permeability carbonates (e.g., micritic limestones). However, primary (e.g., bedding interfaces) and secondary (e.g., fractures) rock planar anisotropies might compensate for this low porosity/permeability, acting as potential pathways for fluid ingress and as loci for the initiation of fluid-rock interaction. Among these anisotropies, burial stylolites are particularly widespread in carbonate successions, forming through progressive chemo-mechanical dissolution-precipitation over time. Their large lateral continuity (>1 km) and potentially high vertical frequency make stylolites key features in governing the syn-to-post diagenetic evolution of sedimentary successions.

Although stylolites have traditionally been considered fluid barriers, recent studies challenge this paradigm, a view that we further stress here. We present petrophysical data from micritic limestones of the Lessini Mountains (Italian Southern Alps), where a large portion of the exposed carbonate Jurassic-Cretaceous succession (>700 m thick) is almost entirely overprinted by a regional dolomitization event, which produced large volumes of massive, sandy, crystalline dolostones. We studied preserved patches of micritic limestone where the progression of dolomitization from initiation to complete overprint is clearly visible. Hg-porosimetry, SEM imaging, μ-CT and cathodoluminescence were combined to constrain petrophysical variations associated with dolomitization. Results show that burial stylolites (Hg injection capillary threshold pressure – HgP c. 4 Psi) affecting the micritic limestones (HgP c. 5140 Psi) were systematically exploited by the dolomitizing Mg-rich fluids, transiently aided by fluid overpressure surges, which locally induced brecciation and further enhanced fluid-rock interaction.

Progressive dolomitization increased rock porosity and density from ~1% to ~20% and from 2.65 g/cm3 to 2.9 g/cm3, respectively (from micritic limestone to massive dolostone). Pore characteristics (pore-size, sphericity, 3D-φ-angle and 3D-Eulerian characteristic - all constrained by μ-CT data and Hg-μporosimetry) indicate a complex evolution characterised by (i) early diffuse dolomitization followed by (ii) localised dedolomitization triggered by the later ingress along the porous stylolites of a Mg-poor fluid, which selectively infiltrated the dolomitized succession and created significant rock porosity. Dedolomitization appears to have been more efficient (and is better preserved) along the dolomitized stylolites than within the massive dolostones, where fluid-rock interaction was inhibited by the larger rock volume.

Spatio-temporal porosity variations related to dolomitization and dedolomitization, guided by- and preserved within stylolites, have significant implications for (i) reservoir quality evaluation, and (ii) the mechanical behaviour of carbonate rock masses during post-fluid-infiltration deformation phases. In these settings, dolomitization and dedolomitization promote long-term fluid ingress and circulation, thus even modulating further deformation localisation.

How to cite: Zuccari, C., Vignaroli, G., Balsamo, F., Berio, L., Buono, G., Pappalardo, L., and Viola, G.: Stylolite-controlled dolomitization and dedolomitization in low-porosity carbonates (Lessini Mountains, Southern Alps, Italy), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14061, https://doi.org/10.5194/egusphere-egu26-14061, 2026.

EGU26-14523 | ECS | Posters on site | TS1.6

Tectono-magmatic controls on fluid flow in a detachment-related porphyry system: Insights from magnetic petrofabric analyses at the Maronia deposit, NE Greece 

Elisa Toivanen, William McCarthy, Daniel Koehn, and Barbara Kleine-Marshall

The circulation of magmatic-hydrothermal fluids along crustal-scale fault systems plays a fundamental role in the formation of porphyry-type ore deposits, as these structures control magma emplacement, fluid pathways, and associated rock alteration. In the Rhodope magmatic-metallogenic belt of northern Greece, numerous Oligocene-Miocene porphyry-type ore deposits formed in an extensional back-arc environment. One example is the Maronia Cu-Mo±Re±Au porphyry deposit in the Mesozoic Circum-Rhodope metamorphic belt, where plutonic intrusion occurred during detachment fault activation. Despite this, the detailed sequence and timing of magmatic-hydrothermal fluid circulation related to ore formation remain poorly constrained.

In this study, we aim to unravel the relationship between magmatic and tectonic events to decipher the mechanisms of magmatic-hydrothermal fluid circulation along detachment faults associated with ore formation processes. A total of 20 rock samples were collected across the exposed detachment fault zone at Maronia, ranging from unaltered monzonite to the porphyry microgranite intrusion. We combined highly sensitive Anisotropy of Magnetic Susceptibility and Remanence (AMS and ARM) petrofabric tools with geochemical analyses (e.g., EPMA, LA-ICP-MS/MS). Petrofabric analyses identified multiple magnetic fabrics within individual samples, providing insights into magmatic intrusion emplacement, deformation, and fluid flow, as well as into whether magmatic and tectonic processes occurred concurrently or successively.

Preliminary geochemical and magnetic analyses of minerals and whole rocks constrain the genetic relationship between microgranite intruding the mylonitic rocks within the detachment fault. Petrofabric data are coaxial with observed field fabrics, whereas preliminary ARM results indicate that higher coercivity mineral phases deviate from both field observations and AMS results. Petrographic observations reveal the nature of mineralization and allow evaluation of textural changes related to fluid-rock interaction. We suggest that the combined dataset reflects a strain archive of multi-stage tectonomagnetic processes that drove fluid flow and possibly mineralisation in this sector of the Circum-Rhodope belt.

This study further demonstrates the potential of integrating petrofabric data with geochemical methods to better resolve fluid flow processes and tectono-magmatic evolution in detachment-controlled porphyry systems, providing new insights into the structural controls on mineralization at Maronia.

How to cite: Toivanen, E., McCarthy, W., Koehn, D., and Kleine-Marshall, B.: Tectono-magmatic controls on fluid flow in a detachment-related porphyry system: Insights from magnetic petrofabric analyses at the Maronia deposit, NE Greece, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14523, https://doi.org/10.5194/egusphere-egu26-14523, 2026.

EGU26-17657 | Posters on site | TS1.6

Fluid-induced strain softening during the formation of the Pyrenean orogenic prism: In situ Rb/Sr dating from the Cap de Creus shear zones (Eastern Pyrenees, Spain) 

Yoann Denele, Clémence Nicolas, Valérie Bosse, Olivier Merle, Emmanuel Gardés, and Caroline Lotout

The aims of this study is to understand how concurrent fluids and deformation influence the behaviour of the Rb/Sr geochronometer in micas. This study is conducted within a classical deformation framework, shear zones, key structures in the geodynamic evolution of rifts and orogens which can accommodate kilometer-scale displacements and facilitate significant mass transfer. While the last two decades have led to a better understanding of the processes of nucleation and widening of these structures, as illustrated by the world-famous case of Cap de Creus, the extreme localization of deformation they exhibit raises fundamental questions about the rheological evolution of the lithosphere.

By conducting a multiscale petro-tecto-geochronological study of the Cap de Creus shear zones, whose age is debated, we have underlined that these shear zones record a major event of fluid-induced strain softening during the formation of the Pyrenean prism. This event is characterized by concomitant muscovite blast neocrystallization and intense quartz dynamic recovery, whose contemporaneity can be uniquely demonstrated by evidence of Fe-rich surface-derived fluids that penetrated to depth. This event occurred between 60 and 50 Ma, as shown by in situ and in-context Rb/Sr dating of two shear zones. This study highlights the critical role of fluid-induced rheological softening in ductile reactivation of polycyclic basements and provides a context-dependent framework for interpreting the behaviour of the Rb/Sr geochronometer in muscovite during deformation.

The implications of these results for the three-dimensional formation and evolution of the Pyrenean orogenic prism, will be discussed, including the role of structural inheritance, fluid circulation, and their contribution to shear-zone reactivation processes.

How to cite: Denele, Y., Nicolas, C., Bosse, V., Merle, O., Gardés, E., and Lotout, C.: Fluid-induced strain softening during the formation of the Pyrenean orogenic prism: In situ Rb/Sr dating from the Cap de Creus shear zones (Eastern Pyrenees, Spain), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17657, https://doi.org/10.5194/egusphere-egu26-17657, 2026.

EGU26-17856 | Posters on site | TS1.6

Tectonics and Fluid Coupling in Critical Metal Enrichment 

Shuyun Cao, Xiaowen Li, Lefan Zhan, Dingkui Zhou, Jianhua Liu, Xuemei Cheng, Lirong Tao, Jing Guo, and Zhongtian Hu

This study investigates the coupled roles of solid-state deformation, hydrothermal fluid flow, and critical metal enrichment mineralization. Integrating structural analysis, mineral microtextures, EBSD, fluid inclusions, and H-O isotopes, we show that the deposit experienced Neoproterozoic Nb pre-enrichment in alkaline volcanic rocks, later overprinted by Early Paleozoic tectonic-hydrothermal events. Ductile shear zones that characterized by foliation and lineatio enhanced permeability and channeled F⁻-Cl⁻-CO₂-rich fluids from deep sources, with fluid inclusion planes confirming foliation-parallel migration. Syn-tectonic breakdown of amphibole, pyroxene, and titanite released Nb, Y, and REEs into solution as soluble complexes.

Fluid evolution—driven by alkali consumption and CO₂ influx, lowered pH and increased Nb solubility. Nb enrichment occurred via water-rock interaction within shear zones, though complex stability initially inhibited precipitation. Localized Nb deposition took place at altered mineral margins, where Fe²⁺ spikes destabilized complexes. Ore bodies formed in brittle–ductile to brittle domains, governed by the interplay of deformation-controlled permeability and chemical feedbacks.

Strain regime shifts further enhanced permeability, enabling mixing between deep NbF6⁻- YF63⁻-CO₂-rich fluids and external alkaline magmatic or Ca-rich fluids. This mixing triggered pH and redox changes that destabilized metal complexes, precipitating Nb minerals as magnetite/ilmenite-hosted inclusions or microveins, which direct evidence of strain and fluid pulsation. Fault-valve cycling induced fluid immiscibility and boiling, further disrupting complex stability. Our findings underscore that tectonically driven fluid migration is fundamental to Nb enrichment, providing a structural framework for exploring orogenic rare-metal deposits.

How to cite: Cao, S., Li, X., Zhan, L., Zhou, D., Liu, J., Cheng, X., Tao, L., Guo, J., and Hu, Z.: Tectonics and Fluid Coupling in Critical Metal Enrichment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17856, https://doi.org/10.5194/egusphere-egu26-17856, 2026.

EGU26-18788 | ECS | Orals | TS1.6

Investigating the Significance of Magnetic Fabrics Preserved in Hydrothermally Altered Rocks 

Ben Latimer, William McCarthy, Tobias Mattsson, and John Reavy

Anisotropy of Magnetic Susceptibility (AMS) and Anisotropy of Magnetic Remanence (AMR) are critical petrofabric tools commonly applied in investigating the evolution of volcano-magmatic, tectonic, and surface process systems. These highly sensitive techniques can distinguish multiple magnetic fabrics within individual samples, shown to be crucial in assessing archives of emplacement and deformation in intrusions where magmatic and tectonic processes occur concurrently or successively. They have also been used to understand magmatic processes within layered igneous complexes associated with the concentration of economic mineral phases. However, the application of AMS and AMR is hindered by the mineral phases that dominate magnetic properties and their susceptibility to hydrothermal alteration, potentially overprinting pre-existing petrofabrics. Despite the impacts of hydrothermal alteration being a well-known occurrence, the mechanisms and extent to which magnetic fabrics can be modified remains poorly constrained, raising concerns about the reliability of interpretations in studies involving hydrothermally altered rocks.

Our recent work assesses the significance of magnetic fabrics preserved in a hydrothermally altered fault zone that crosscuts a granitic pluton. Data were collected from unaltered granodiorite peripheral to the fault, the fault damage zone and the fault core to assess the impact of hydrothermal alteration on magnetic fabrics associated with magmatic and tectonic processes. Magnetic and hyperspectral data were used to characterise alteration distribution and intensity by quantifying changes in hydrous silicate and iron oxide phases. AMS and AMR fabrics were then measured and interpreted as either magma transport, tectonic, or hydrothermal alteration fabrics with context from field and petrographic data.

Our integrated hyperspectral-magnetic approach defines three alteration zones. Onset of hydrothermal alteration is identified from a subtle removal of white mica and low coercivity iron oxides (titanomagnetite) and the growth of new, high coercivity iron oxides (hematite) alongside chlorite and epidote. As alteration intensity increases, titanomagnetite and white mica are removed entirely, with hematite, epidote and chlorite becoming dominant in the system. In step with the changes in oxide and hydrous silicate mineralogy, we observe changes to AMS and AMR fabrics, with partial to complete destruction of tectonic and magmatic fabrics observed with increased alteration intensity. As these precursor fabrics are destroyed, they are replaced by a sub-vertical petrofabric defined by the alignment of hematite, interpreted as a product of hydrothermal fluid transport.

We demonstrate a threshold to alteration intensity, above which precursor petrofabrics are obliterated and replaced by fabrics associated with hydrothermal alteration. We envisage these results being highly informative in studies seeking to examine tectonic and mineralisation processes using rock magnetic methods.

How to cite: Latimer, B., McCarthy, W., Mattsson, T., and Reavy, J.: Investigating the Significance of Magnetic Fabrics Preserved in Hydrothermally Altered Rocks, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18788, https://doi.org/10.5194/egusphere-egu26-18788, 2026.

EGU26-20074 | Posters on site | TS1.6

Permeability anisotropy under true triaxial stress states: strong flow reduction parallel to the maximum principal stress. 

Philip Meredith, Ashley Stanton-Yonge, Thomas Mitchell, John Browning, and David Healy

Rocks in the upper crust are generally subjected to true triaxial stress conditions, in which all three principal stresses are unequal (σ₁ > σ₂ > σ₃). Pore and fracture networks respond to anisotropic loading by opening in certain directions while closing in others, potentially inducing strong permeability anisotropy. However, most experimental constraints on stress-dependent permeability are derived from conventional triaxial tests, where two principal stresses are equal and permeability is measured in only one direction.

Here, we use a true triaxial apparatus equipped with a pore-fluid system to measure permeability parallel to all three principal stress axes in cubic samples of Etna basalt (EB) and Crab Orchard sandstone (COS) subjected to anisotropic loading.

For an initially isotropic EB sample, increasing stress along a single axis results in a sharp permeability decrease in the corresponding maximum stress direction, reaching up to two orders of magnitude (from ~10⁻¹⁶ to ~10⁻¹⁸ m²) at a differential stress (σ₁ − σ₃) of 215 MPa. In contrast, permeability parallel to σ₂ decreases mildly when stresses are increased up to ~75 MPa while permeability parallel to σ₃ remains largely unchanged. During unloading, permeability parallel to σ₁ recovers by approximately 1.5 orders of magnitude once σ₁ is reduced to 75 MPa.

Similarly, samples of the initially anisotropic COS also experience a decrease in permeability of two orders of magnitude (from ~10⁻¹7 to ~10⁻¹9 m²) along the maximum compressive stress at (σ₁ − σ₃) of just 100 MPa. Permeability along σ₁ recovers only partially after unloading, up to 10⁻¹8 m², indicating that some permanent compaction occurred along the maximum compression.

These results demonstrate that true triaxial stress conditions can induce pronounced permeability anisotropy through directional closure of pores and microcracks, with important implications for fluid transport in the upper crust, including fault zones, geothermal systems, and stressed reservoirs.

How to cite: Meredith, P., Stanton-Yonge, A., Mitchell, T., Browning, J., and Healy, D.: Permeability anisotropy under true triaxial stress states: strong flow reduction parallel to the maximum principal stress., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20074, https://doi.org/10.5194/egusphere-egu26-20074, 2026.

Graphite formation in deep crust during granulite facies metamorphism is documented in the Proterozoic gneisses of the Lofoten-Vesterålen Complex, northern Norway. Regionally distributed graphite zones are hosted in banded gneisses dominated by orthopyroxene-bearing quartzofeldspathic gneiss, including marble, calcsilicate rocks and amphibolite. The schist has major graphite, quartz, plagioclase, pyroxenes, biotite (Mg# = 0.67-0.91; Ti < 0.66 a.p.f.u.) and K-feldspar/perthite. Pyroxene is orthopyroxene (En69-74) and/or clinopyroxene (En33-53Fs1-14Wo44-53). Although graphite is usually described in pelitic rocks or as vein deposits in the granulite facies rocks, we document graphite in assemblage with metamorphic orthopyroxene.

Phase diagram modelling (plagioclase + orthopyroxene (Mg#-ratio = 0.74) + biotite + quartz + rutile + ilmenite + graphite-assemblage) constrains pressure-temperature conditions of 810-835 °C and 0.73-0.77 GPa; Zr-in-rutile thermometry 726-854°C. COH-fluids stabilise graphite and orthopyroxene; high Mg#-ratio of biotite and pyroxenes, and apatite Cl < 2 a.p.f.u. indicate importance of fluids during metamorphism.

Stable isotopic δ13Cgraphite in the graphite schist is -38 to -17‰; δ13Ccalcite of marbles +3‰ to +10‰. Samples with both graphite and calcite present give lighter values for δ13Ccalcite = -8.7‰ to -9.5‰ and heavier values for δ13Cgraphite = -11.5‰ to -8.9‰. δ18Ocalcite for marble shows lighter values ranging -15.4‰ to -7.5‰ (Engvik et al. 2023).  We interpret the graphite origin as organic carbon accumulated in sediments contemporaneous with the Early Proterozoic global Lomagundi-Jatuli isotopic excursion, while an isotopic exchange between graphite and calcite reflects metamorphic and hydrothermal re-equilibration.

The high-ordered graphite (< modality 39%) and biotite with a strong-preferred orientation defines the well-developed foliation. Increased graphite content resulted in high-conductivity zones with a contrast to the host low-conductive crust (Rodinov et al. 2013; Engvik et al. 2021). Enrichment of graphite resulted in zones with strong schistosity and a sharp strain gradient towards host massive granulite gneiss. The presence of graphite causes strain localisation in the granulite facies crust, reducing crustal strength and may thereby influence continental architecture and evolution of collision zones.

References:

Engvik AK et al. (2023) Proterozoic Deep Carbon—Characterisation, Origin and the Role of Fluids during High-Grade Metamorphism of Graphite (Lofoten–Vesterålen Complex, Norway). Minerals 13(10), 1279

Engvik AK et al. (2021) The control of shear-zone development and electric conductivity by graphite in granulite: An example from the Proterozoic Lofoten-Vesterålen Complex of northern Norway. Terra Nova, https://doi.org/10.111/ter.12545

Rodinov A et al. (2013) Helicopter-borne magnetic, electromagnetic and radiometric geophysical survey at Langøya in Vesterålen, Nordland. NGU Report 2013.044

How to cite: Engvik, A. K., Gautneb, H., and Knežević Solberg, J.: Characterisation, origin, petrophysical properties and the role of fluids during high-grade metamorphism of graphite (Lofoten-Vesterålen Complex, Norway), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21791, https://doi.org/10.5194/egusphere-egu26-21791, 2026.

Volcanogenic massive sulfide (VMS) deposits are among the world’s most important sources of copper (Cu), zinc (Zn), lead (Pb), gold (Au), and silver (Ag), metals that are critical for modern infrastructure and energy technologies. These deposits are characterized by systematic hydrothermal alteration halos that preserve mineralogical and chemical gradients generated by spatial and temporal variations in temperature, redox conditions, and hydrothermal fluid composition. Such alteration zones provide important vectors for mineralization; however, their traditional characterization is commonly qualitative, reliant on subjective geological interpretation, and difficult to collolate at scale across exploration projects. This study investigates the Rävliden deposits of the Paleoproterozoic (1.89 Ga) volcanic–sedimentary sequence of the Skellefte district, Sweden, to evaluate whether integrated rock magnetic and VNIR–SWIR hyperspectral data can be used to objectively characterize hydrothermal alteration in VMS deposits. In this study, rock magnetic measurements are cross-referenced with hyperspectral data and supported by mineral chemistry and sulfur isotope analyses to develop a quantitative and reproducible framework for fingerprinting hydrothermal alteration in both metalliferous and barren VMS systems. The approach comprises three objectives: (1) defining diagnostic magnetic and hyperspectral signatures of alteration mineral assemblages to construct a reference dataset, which is then validated using Raman spectroscopy; (2) evaluating trace-element variations in magnetite and associated sulfide minerals to assess their influence on magnetic properties across alteration zones; and (3) using sulfur isotope compositions (δ³⁴S) of sulfide minerals across alteration zones and structural domains to constrain fluid sources and reconstruct the hydrothermal fluid evolution of the system. This workflow systematically links observable physical alteration patterns to their underlying mineral-chemical controls and fluid origins, providing a robust and scalable tool for hydrothermal alteration characterization in VMS exploration.

How to cite: Aryani, L. and McCarthy, W.: Integrated Rock Magnetic and VNIR–SWIR Hyperspectral Characterization: A Quantitative Classification Tool for VMS Alteration Systems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22148, https://doi.org/10.5194/egusphere-egu26-22148, 2026.

EGU26-22152 | ECS | Posters on site | TS1.6

Go with the Flow : Investigating Petrofabric Evidence for Hydrothermal Flow in Thermal Aureoles 

Malou Pelletier and William McCarthy

Fluid flow in the Earth’s crust governs heat and mass transfer, critical metal mineralisation, rock rheology, and the development of deep, non-photosynthetic biospheres, yet its direction and mechanical drivers remain poorly constrained in natural systems. Conventional approaches infer fluid pathways from fractures, models, or geochemical tracers but rarely capture flow direction or mechanism directly. This PhD project develops a novel combination of fabric-based methods—integrating anisotropy of magnetic susceptibility and remanence (AMS/ARM), crystal preferred orientation analysis, and hyperspectral mineral mapping—to directly identify and quantify fluid-induced petrofabrics within the thermal aureoles of igneous intrusions, independent of fault kinematics. Similar integrated approaches have demonstrated their ability to track volatile-rich liquid migration through texturally layered intrusions, where permeability contrasts control fluid focusing and the development of REE-enriched horizons. Together, these methods provide new constraints on how fluids modify host-rock properties, localise permeability, and generate chemical enrichment, representing a step-change in our ability to observe and model crustal fluid flow.We present new petrofabric data from the Sherwood Sandstone Group, Northern Ireland, to assess fluid flow in permeable sandstones surrounding basaltic dykes. The study examines: (i) the geometry and extent of hydrothermal flow pathways, (ii) the interaction between thermally driven fluid circulation and pre-existing sedimentary anisotropy, and (iii) the impact of alteration on host-rock porosity and permeability. The Sherwood Sandstone Group forms the lowermost unit of the Triassic New Red Sandstone succession and is cross-cut by Palaeogene basaltic dykes related to North Atlantic rifting. Preliminary field observations and hyperspectral data identify laterally zoned alteration halos defined by systematic variations in clay, mica, and Fe-oxide mineralogy. AMS and ARM data reveal that primary sedimentary fabrics are preserved more than ~10 m from the dyke but are progressively overprinted toward the intrusion. Ongoing analyses test whether these overprinting fabrics record convective hydrothermal flow, with fluids ascending along dyke margins before dispersing laterally along bedding planes. We further evaluate the controls on stratigraphic fluid focusing and blockage, constraining the reciprocal relationship between fluid flow and evolving rock properties.

How to cite: Pelletier, M. and McCarthy, W.: Go with the Flow : Investigating Petrofabric Evidence for Hydrothermal Flow in Thermal Aureoles, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22152, https://doi.org/10.5194/egusphere-egu26-22152, 2026.

EGU26-394 | ECS | Orals | TS3.3

Inhomogeneity of East-West Extension Interior of the Tibetan Plateau 

shiguang wang, Paul Tapponnier, Marie-Luce Chevalier, Lucilla Benedetti, and Xiwei Xu

Holocene slip rates of active faults are critical to understand the kinematics of crustal deformation interior of the Tibetan Plateau. Here, we quantitatively studied the sinistral strike-slip rate the northern Yadong-Gulu rift (YGR), the unique one that has left-lateral component among the main seven N-S treading rifts in southern Tibet. By detailed fieldwork, UAV topographic data and 10Be cosmogenic dating, we document 2.5-3.5 mm/yr (3.0±0.5 mm/yr) Holocene left-lateral slip rate along the northern YGR at two moraine sites. This rate is consistent with GPS results (4 mm/yr) of the conjugate strike-slip faults in central Tibet. Both of this fault and the northern Beng Co dextral strike-slip fault (4.2-5.4 mm/yr) probably comprise a conjugate fault system, contributing to the extension rate of Gulu rift (~6±1.8 mm/yr) and accommodating the eastward extrusion of central Tibet.  

How to cite: wang, S., Tapponnier, P., Chevalier, M.-L., Benedetti, L., and Xu, X.: Inhomogeneity of East-West Extension Interior of the Tibetan Plateau, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-394, https://doi.org/10.5194/egusphere-egu26-394, 2026.

EGU26-2143 | Posters on site | TS3.3

New Slip Rate of the Central Gulang-Zhongwei Fault determined from high resolution topography and, OSL and 14C dating 

Boming Li, Yanxiu Shao, Yunsheng Yao, Huixin Zhang, and Yu Dong

    The Gulang-Zhongwei Fault is a northeast splay of the Haiyuan fault (east of 102°E) accommodating mostly left-lateral slip and some thrusting. Its slip history and kinematics are critical for understanding the mechanisms of slip partitioning along the oblique convergence at the margin of the plateau. Up to now, a consensus on its slip rate remains elusive; previous investigations have yielded divergent estimates ranging from <1 to 6 mm/yr. The central segment of the Gulang–Zhongwei Fault has been targeted for a detailed geomorphological and paleoseismological study. We used drone-based lidar to collect aerial imagery and dense point cloud to generate a digital elevation model (DEM) with a spatial resolution of better than 6 cm. The DEM clearly reveals the fault trace with faulted geomorphic features such as offset terraces and alluvial fans along the southern piedmont of Jingtai Xiaohongshan and Guanguan Ling . We performed detailed geomorphological mapping and displacement measurements at five sites over a fault length of ~6 km. The initiation time of fault slip accumulation was constrained by sub-surface 14C and OSL dating of various terraces and fan surfaces. Systematic and repeated offsets of multiple alluvial fans and terraces, with an average displacement of 12 m, postdating their emplacement in the early Holocene (8–10 ka), imply a millennial slip rate of 0.9–1.5 mm/yr. Altogether, our results indicate that the long-term left-lateral strike-slip rate of the Gulang-Zhongwei Fault ranges from 0.9 to 1.5 mm/yr. Although it accommodates only 10 % to 15 %of the left-lateral shear between Gobi-Ala Shan to the north and northeast Tibet to the south, it has been responsible for some major earthquakes in the past (1709 and 1920). Determination of its slip rate at various time scales is paramount for understanding how northeast convergent strain is distributed along the various faults at the regional scale and is key to seismic hazard assessment.

How to cite: Li, B., Shao, Y., Yao, Y., Zhang, H., and Dong, Y.: New Slip Rate of the Central Gulang-Zhongwei Fault determined from high resolution topography and, OSL and 14C dating, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2143, https://doi.org/10.5194/egusphere-egu26-2143, 2026.

EGU26-2652 | ECS | Posters on site | TS3.3

Deformation mechanism transitions during the seismic cycle recorded by quartz CPO in fault-related silica layers 

Dohee Gu, Raehee Han, André Niemeijer, Daeyeong Kim, Vladimir Roddatis, and Anja Schreiber

Silica layers composed of quartz grains typically a few micrometers or smaller are texturally distinct from typical quartz veins and occur as μm- to mm-thick layers along fault slip zones. The ultrafine quartz within these layers exhibits uniform interference colors in optical microscopy. Such features are commonly interpreted as indicating crystallographic preferred orientation (CPO), a fabric typically associated with ductile deformation but developed within brittle fault zones. Despite their widespread occurrence in faults developed in various rock types, the deformation mechanisms and ultrafine quartz CPO-forming mechanisms through the seismic cycle remain poorly understood.

In this study, we analyze the microstructures of silica layers observed in three upper crustal faults in Korea developed in sedimentary rocks, granite, and rhyolite within the Cretaceous Gyeongsang Basin, where average burial depths reach ~6 km. All observed natural silica layers are composed of fine-grained quartz (<2 μm. These layers display uniform interference colors in optical microscopy, while EBSD analyses reveal clustering of quartz c-axes. However, some faults are characterized by densely packed comminuted grains with nanopores, whereas others display polygonal quartz grains together with nanopores and illite aligned parallel to the fault plane, as well as shape-preferred orientation of quartz and adjacent calcite grains. These observations suggest that ultrafine quartz within silica layers may have experienced diffusion-related processes in the presence of fluids.

To investigate whether diffusional processes active after fault slip and cataclasis affect CPO development, we conducted hydrothermal rotary shear experiments on single-crystal quartz gouge (<63 μm) under identical P-T-fluid conditions (600°C, effective normal stress of 120 MPa, pore fluid pressure of 80 MPa) using three different velocity histories: (1) fast slip alone (V=300 μm/s), (2) fast slip followed by slow slip (V=0.1 μm/s), (3) fast slip followed by hydrothermal holding without further shear (22 h). The fast slip produces intense comminution within slip localized zones without the development of CPO-like features. In contrast, both the subsequent slow slip and hydrothermal holding result in the development of CPO-like features at the optical scale within the grain-size-reduced zones, accompanied by surface indentations on larger quartz grains and linear aggregates of euhedral ultrafine quartz. However, TEM observations reveal that ultrafine quartz grains within these zones display random crystallographic orientations, with no evidence for a preferred orientation.

Integrating natural and experimental observations, we interpret silica layers to form through a two-stage process: intense grain-size reduction by comminution during seismic slip, followed by fluid-assisted, time-dependent reorientation of ultrafine quartz during post-seismic or interseismic periods. Silica layers characterized by CPO-like features at the optical scale therefore record transitions in deformation mechanisms during the seismic cycle and provide key geological constraints for understanding slip behavior, mechanical properties, and the role of fluids in upper crustal faults. Further investigation is required to clarify the relationship between these optical features and crystallographic orientations at the nanoscale.

How to cite: Gu, D., Han, R., Niemeijer, A., Kim, D., Roddatis, V., and Schreiber, A.: Deformation mechanism transitions during the seismic cycle recorded by quartz CPO in fault-related silica layers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2652, https://doi.org/10.5194/egusphere-egu26-2652, 2026.

EGU26-3578 | ECS | Posters on site | TS3.3

Cohesion-driven fault instability 

Giuseppe Volpe, Raphael Affinito, Giacomo Pozzi, and Cristiano Collettini

Fault healing is a fundamental process in the seismic cycle, allowing faults to relock and restrengthen during the interseismic period. Numerous geophysical studies have shown that the rate of fault healing plays a key role in controlling both earthquake magnitude and recurrence interval, in laboratory experiments as well as in natural fault systems. At the laboratory timescales (1–10⁵ s), fault healing is predominantly frictional and results from the time-dependent growth of contact area due to plastic deformation of the contact asperities. In contrast, seismic cycles in nature occur over much longer timescales, allowing additional healing mechanisms, often driven by chemically assisted processes, to become dominant.

Field observations reveal that chemically cemented fault rocks, such as cataclasites, are commonly present within the cores of several exhumed faults. Despite their widespread occurrence, the interplay between chemically-driven healing processes and fault stability remains poorly constrained by laboratory studies, largely due to the limited experimental timescales.

Here we present a suite of laboratory friction experiments specifically designed to overcome these limitations. We use analogue fault gouges composed of highly reactive materials, including hydraulic cement and anhydrite, tested under both nominally dry and fluid-saturated conditions. This approach allows us to investigate the combined and competing effects of frictional and chemically driven healing on fault slip behavior.

Microstructural and geochemical analyses reveal the formation of newly precipitated mineral phases under fluid-saturated conditions, consistent with the expected reaction for both gouge materials. Compared to purely frictional healing, chemically driven healing produces larger, non-log-linear fault restrengthening and a time-dependent increase in fault cohesive strength. Moreover, faults undergoing chemically driven healing exhibit unstable fault slip, characterized by recurrent stick–slip cycles.

These results indicate that chemically-driven healing processes play a fundamental role in interseismic fault restrengthening and may critically influence fault stability over geological timescales. Our results also suggest that these chemically-driven healing processes may favor the development of favorable conditions for unstable slip even at shallow depths, with relevant implications for natural and induced seismicity.

 

How to cite: Volpe, G., Affinito, R., Pozzi, G., and Collettini, C.: Cohesion-driven fault instability, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3578, https://doi.org/10.5194/egusphere-egu26-3578, 2026.

EGU26-4687 | Posters on site | TS3.3

Internal Structure and Kinematic Evolution of the Hambaeksan Fault, Taebaeksan Basin, South Korea 

Jae Hoon Kim, Jin-Han Ree, Raehee Han, and Jusun Woo

The Hambaeksan Fault is a major structural feature in the Taebaeksan Basin, South Korea, characterized by a significant right-lateral strike separation of approximately 3–5 km. Although it truncates the Baekunsan Syncline, the precise timing and kinematic history of the fault remain poorly understood. This study investigates the internal structures, fault rock characteristics, and kinematic indicators of the Hambaeksan Fault through field observations and microstructural analysis at the Sorotgol road outcrop in Taebaek.

At the study site, the fault juxtaposes the limestone of the Duwibong Formation against the shale of the Geumcheon-Jangseong Formation. The fault zone strikes N-S with a 65°E dip, comprising a ~30 cm thick fault core and a damage zone exceeding 10 m. The fault core consists of limestone breccia, shale breccia, and mixed breccia. Linear structures within the shale breccia (N5°E, 10°) confirm a dominant strike-slip movement.

Microstructural analysis reveals a complex deformation history characterized by several distinct features. A well-defined, linear Principal Slip Zone (PSZ), approximately 300 μm thick, is developed within the shale breccia and sharply truncates earlier clasts. Within the mixed breccia, the presence of clay-rich matrices exhibiting fluidized textures and injection structures suggests the occurrence of seismic slip, possibly involving rapid fluidization. Furthermore, kinematic overprinting is evident in the shear bands adjacent to the PSZ, where sinistral shear senses are superimposed on earlier dextral shear senses. These observations indicate that the Hambaeksan Fault has experienced a multi-stage evolution, beginning with a primary dextral strike-slip movement followed by localized subsequent deformation within the mechanically weaker shale units.

These findings suggest that the Hambaeksan Fault underwent at least one episode of seismic slip along the lithological boundaries (mixed breccia) prior to the formation of the current PSZ in the shale unit. The observed kinematic overprinting indicates that after the initial juxtaposition of the formations via dextral strike-slip movement, subsequent deformations were localized within the mechanically weaker Geumcheon-Jangseong shale. This study provides critical insights into the seismic behavior and structural evolution of major crustal faults in the Korean Peninsula.

How to cite: Kim, J. H., Ree, J.-H., Han, R., and Woo, J.: Internal Structure and Kinematic Evolution of the Hambaeksan Fault, Taebaeksan Basin, South Korea, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4687, https://doi.org/10.5194/egusphere-egu26-4687, 2026.

EGU26-5101 | Posters on site | TS3.3

Slip partitioning of the Altyn Tagh fault based on geomorphic indices reveals uplift pattern 

Mingxing Gao, Jerome van der Woerd, and Juntao Cai

Active strike-slip fault systems in addition to oblique slip producing vertical displacement are often linked to contemporaneous thrust faults, which together contribute to regional uplift. However, how slip is partitionned along the different faults of the strike-slip fault system and the underlying mechanisms of slip-paretionning remain poorly understood. To address this issue, we investigated the northwestern margin of the Tibetan Plateau, focusing on the Altyn Tagh fault—a complex fault system that has undergone major Cenozoic tectonic deformation due to the ongoing convergence between the Indian and Asian plates. Using drainage networks and geomorphic indices, we developed a composite index of Relative Uplift Rate (RUR) to map spatial variations in uplift rates. Our analysis reveals significant along-strike variations in tectonic uplift and identifies four major tectonic anomalies from south to north: Qiemo, Subei, Changma, and the northern Qilian Shan. By integrating these results with geological constraints on horizontal slip rates, we explore the mechanism of slip partitioning along the fault. We find that although horizontal slip rates generally decrease northeastward, the vertical relative uplift rates do not follow the same pattern. Instead, within the Qilian Shan, vertical uplift rates are the highest compared to the southwestern fault junction areas. A key finding is that areas with high uplift rates correspond spatially to zones of geometrical fault complexity, such as fault bends or branching. These anomalies are further supported by patterns of seismic activity.

How to cite: Gao, M., van der Woerd, J., and Cai, J.: Slip partitioning of the Altyn Tagh fault based on geomorphic indices reveals uplift pattern, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5101, https://doi.org/10.5194/egusphere-egu26-5101, 2026.

EGU26-5279 | ECS | Orals | TS3.3 | Highlight

The effect of frictional heterogeneities on the seismic cycle: Insights from triaxial experiments 

Corentin Noël, Pierre Dublanchet, Cédric Twardzik, and François Passelègue

Deformation within the upper crust is mainly accommodated through slip on fault systems. Slip can occur in various forms, ranging from aseismic creep (i.e., stable motion) to dynamic earthquake (i.e., unstable motion). Interestingly, a single fault is not restricted to a specific slip mode. Recent geodetic observations have shown that a fault can exhibit both stable and unstable motions. The different slip behaviours have been attributed to fault spatial heterogeneity of the frictional properties, rheological transitions, or geometric fault complexity.

To comprehensively characterise the effect of frictional heterogeneities, we deformed heterogeneous fault samples in a triaxial apparatus, at confining pressures ranging from 30 to 90 MPa. The fault planes, sawcut at a 30° angle from the sample axis, are composed of two materials: granite and marble. Experiments were conducted with both marble asperities embedded in granite and vice versa, alongside homogeneous fault samples of single lithology. The selection of granite and marble was based on their different frictional properties, with granite exhibiting seismic behaviour, while marble demonstrated aseismic behaviour under the tested conditions.

Our results show that the stress drops of seismic events are dependent on fault composition, with faults containing higher granite content exhibiting larger stress drops. In addition, local strain measurements close to the fault allow us to investigate the spatial and temporal distribution of fault slip. In the case of homogeneous faults, the seismic event nucleation is relatively straightforward, initiating in the highest stressed region and propagating uniformly. Conversely, heterogeneous faults display a shorter nucleation phase, followed by a dynamic strain drop restricted close to the granite areas. Away from the dynamic event, the fault remains locked and is subjected to an increase in strain. This strain deficit is then released by a long-lasting decay similar to post-seismic afterslip observed on natural fault systems after large earthquakes. For the heterogeneous samples exhibiting post-seismic deformation, elevated confining pressure favours longer and higher amplitude of afterslip. Further data analysis demonstrated that large afterslip observed at higher confining pressures must originate from the combination of 1) larger co-seismic stress/strain drop and 2) higher frictional stability around the area of dynamic stress/strain drop, both enhanced at larger confining pressures.

How to cite: Noël, C., Dublanchet, P., Twardzik, C., and Passelègue, F.: The effect of frictional heterogeneities on the seismic cycle: Insights from triaxial experiments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5279, https://doi.org/10.5194/egusphere-egu26-5279, 2026.

Unlike typical surface rupture zones that develop along the main fault of mainshocks, the January 23, 2024, Wushi earthquake in Xinjiang, despite its magnitude of Mw 7.0 and relatively shallow focal depth of 22 km, did not produce any co-seismic surface rupture along the seismogenic South Maidan Fault (SMDF). Instead, seven days later, an Mw 5.7 aftershock along a reactivated shallow back-thrust occurred approximately 3.7 km northwest of the SMDF, generating a co-seismic surface rupture about 4.7 km long. Together, these two faults form a pop-up structure with opposite vergence, triggered by the aftershock thus causing significant and localized surface uplift. This unusual case offers new insight into faulting dynamics, landscape evolution, and underscores the need to reassess the seismic hazard posed by shallow secondary faults.

On the rupture surface, a layer of red fault gouge approximately 0.5–1 cm thick has developed. Outward from this, there is a layer of light yellow fault breccia about 20–30 cm thick. A clear linear boundary exists between the two, and the entire assemblage is enclosed within a fragmented zone composed of Xiyu conglomerate. We combined rupture energy, δD, the Kübler index parameter, and multi-grain-size structural analyses with K-Ar dating of synkinematic illite separated from both the red fault gouge and surrounding fault breccia rocks.

The dating results show that the red fault gouge records a new round of strong earthquake clusters beginning at 0.34 ± 0.03 Ma. The detrital illite age was 2.04 ± 0.13 Ma, which is consistent with the sedimentary age of the Xiyu conglomerates. In contrast, the surrounding yellow-breccia rocks obtain an older clay mineral ages: the authigenic illite age is 204.0 ± 5.8 Ma and the detrital illite age is 419.4 ± 23.6 Ma. Considering that the Xiyu Conglomerate was deposited during the Late Cenozoic and exhibits relatively poor diagenetic consolidation, the terminal ages of its clay minerals likely represent two distinct periods: the initial collision and orogenic phase of the South Tianshan during the Late Silurian to Early Devonian, and a distal response to the closure of the Tethys Ocean during the Indosinian period.

Our findings confirm that the South Tianshan region has entered a new phase of tectonic activity since the Quaternary. Intense crustal shortening triggered extensive erosion, leading to widespread faulting activities and the deposition of the Xiyu conglomerates. By the Middle Pleistocene, back-thrust faults developed as stress accumulated, forming pop-up structures that controlled regional uplift and landscape evolution. These shallow, low-energy secondary faults are still capable of generating surface ruptures during seismic events, and carries important implications for seismic hazard assessment, particularly regarding surface deformation risk.

How to cite: Zheng, Y.: K-Ar dating of fault gouge from the surface rupture of the January 23, 2024 Ms7.1 Wushi Earthquake, Xinjiang, China, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5332, https://doi.org/10.5194/egusphere-egu26-5332, 2026.

EGU26-5564 | Posters on site | TS3.3

Reassessment of the Carboneras Fault 3D geometry based on new bathymetric and high-resolution multi-channel seismic reflection data 

Nathalia Mattos, Hector Perea, Sara Martínez-Loriente, and Ariadna Canari

The NE-SW Carboneras Fault is one of the main active structures in the Alborán Sea and, together with the Al-Idrisi Fault, forms the Trans-Alborán Shear Zone, which connects the Betic and Rif Cordilleras. The accurate representation of the offshore 3D geometry and seismogenic characteristics (e.g., slip rate or maximum magnitude) of this large left-lateral strike-slip fault system is essential for assessing the seismic potential in a slow-deforming region, such as the Alborán Sea. Here, we combine the interpretation of multibeam bathymetric and high-resolution multi-channel seismic reflection (HR-MCS) data to reassess the offshore extent of the Carboneras Fault and the adjacent morphostructural elements. Topographic attributes were applied to the bathymetric data to enhance the visualization of the fault trace at the seafloor. Our findings suggest that the offshore Carboneras Fault extends for 110.3 km, exceeding previous estimates. We identified twenty fault segments along the Carboneras Fault trace, with individual lengths up to 46 km and azimuths varying from N40º to N238º. Geomorphic features typically associated with strike-slip systems such as deflected drainage systems, shutter and pressure ridges, and horsetail splays were also identified. Structural seismic attributes applied to the HR-MCS profiles highlight major subsurface discontinuities, allowing detailed mapping of the fault geometry at depth. Seismic interpretation also accounted with the identification of seven horizons offset by the Carboneras Fault, comprising the Paleozoic-Triassic basement, the Messinian unconformity and Early Pliocene to Late Quaternary seismic units. Based on this information, we constructed fault and horizon surfaces to develop the first 3D model of the Carboneras Fault. This model provides key constraints on crustal architecture and offers new insights into fault growth mechanisms, thereby reducing uncertainties and improving the assessment of the seismogenic potential of this major offshore fault system.

How to cite: Mattos, N., Perea, H., Martínez-Loriente, S., and Canari, A.: Reassessment of the Carboneras Fault 3D geometry based on new bathymetric and high-resolution multi-channel seismic reflection data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5564, https://doi.org/10.5194/egusphere-egu26-5564, 2026.

EGU26-5619 | ECS | Posters on site | TS3.3

Coulomb-like creeping segment acts as a stress sensor in Northern Sumatra 

Sharadha Sathiakumar, Rino Salman, Rishav Mallick, Lujia Feng, Qiang Qiu, Susilo Susilo, Sidik Tri Wibowo, Emma Hill, and Sang-Ho Yun

Understanding the spatial and temporal evolution of creep along continental faults is key to identifying where stress is released aseismically and where it may accumulate, potentially leading to future seismic events. Typically, creeping segments exhibit rate-strengthening behaviour, where frictional resistance increases with sliding velocity, resulting in stable sliding. However, the northern Aceh segment of the Sumatran Fault Zone (SFZ), a right-lateral strike-slip fault, presents a notable exception. Here, we observe creep signals using satellite radar interferometry, capturing the temporal evolution of creep, which decreased by ~60% from the 2007–2010 period to the 2017–2023 period. Numerical modelling constrained by these observations identifies two distinct creep events. The first was triggered by stress transfer from Mw 9.2 2004 earthquake more than 150 km away, and a second localized re-acceleration due to nearby continental earthquakes. These results reveal that the fault behaviour is more consistent with a brittle Coulomb surface and lacking the usual self-stabilizing influence of velocity- and slip history-dependent friction. This central creeping section, sandwiched between two large locked domains, instead exhibits nearly velocity-neutral behaviour at the fault segment scale, making it highly sensitive to both local and regional stress changes. These findings provide evidence of long-range fault interactions, where both the subducting megathrust and possibly the oceanic mantle drive creep on a continental strike-slip fault. Located within a densely populated region, the velocity-neutral Aceh fault may participate in future earthquakes nucleating in surrounding locked segments, highlighting elevated seismic hazard in northern Sumatra.

How to cite: Sathiakumar, S., Salman, R., Mallick, R., Feng, L., Qiu, Q., Susilo, S., Wibowo, S. T., Hill, E., and Yun, S.-H.: Coulomb-like creeping segment acts as a stress sensor in Northern Sumatra, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5619, https://doi.org/10.5194/egusphere-egu26-5619, 2026.

EGU26-6931 | ECS | Orals | TS3.3

Seismicity driven by rapid fault cementation in tuffs under hydrothermal conditions of the Campi Flegrei caldera (Italy) 

Gianluca D'Ippolito, Telemaco Tesei, Angela Mormone, Rodrigo Gomila, Monica Piochi, and Giulio Di Toro

Volcanic calderas, including Campi Flegrei (Italy), are characterized by intense shallow seismicity (<4 km depth, magnitude <4), commonly associated with hydrothermal fluid circulation. In these settings, seismogenic volumes constitute highly reactive systems where pressurized fluids, elevated temperatures, and mineral reactions interact to modulate fault strength, wall rock and fault zone stiffness, and slip behavior (i.e., from aseismic creep to seismic slip). Despite the dense monitoring network at Campi Flegrei—one of the most active and densely populated volcanic–geothermal systems worldwide—the mechanical and chemo-textural behavior of shallow faults under hydrothermal conditions and its implications for the seismic cycle remain poorly constrained.

Here, we investigate the coupled mechanical, mineralogical, geochemical, and microstructural evolution of experimental faults composed of Neapolitan Yellow Tuff, a highly reactive pyroclastic rock representative of the shallow (<1 km) intra-caldera faulted volume at Campi Flegrei. We performed fourteen hydrothermal rotary-shear experiments at constant slip velocity (10 µm s⁻¹), systematically varying temperature (T = 23–400 °C), effective normal stress (σeff = 5–30 MPa), and pore-fluid pressure (Pf = 5–30 MPa) to reproduce liquid, vapor, and supercritical water conditions expected within the upper ~2 km of the caldera. Slip stability was assessed from the occurrence of stick–slip events (laboratory earthquakes), and associated stress drops, while friction coefficients and apparent fault stiffness were retrieved from stick-slip cycles. Mechanical observations were complemented by post-mortem mineralogical, geochemical, and microstructural analyses using X-Ray Diffraction, X-Ray Fluorescence, Fourier Transform Infrared Spectroscopy, Scanning Electron Microscopy, and Energy Dispersive System microanalysis (XRPD, XRF, FTIR, SEM–EDS).

At room temperature, deformation is dominated by stable or slow slips associated with distributed grain-size reduction and limited induration. With increasing temperature, thermally activated mineral reactions alter fault rheology (and behavior). Between 300 and 400 °C, zeolite dehydration, clay dehydroxylation, volcanic glass dissolution, and rapid secondary mineral precipitation promote pervasive cementation and pore-space sealing, producing a dense, welded fault fabric. These processes strengthen grain-to-grain contacts, increase friction coefficients (from ~0.67 at room temperature to ~0.84 at 400 °C), and significantly enhance fault stiffness (from ~2.5 GPa/m at 23 °C up to ~10 GPa/m at 400 °C), leading to strongly unstable, earthquake-like slip with laboratory stress drops of up to ~25 MPa. Increasing effective normal stress further amplifies frictional instabilities through compaction, strain localization, and strengthening of grain contact junctions. In contrast, vapor-dominated conditions at ≥300 °C inhibit cementation, resulting in smaller stress drops while maintaining unstable fault slip behavior.

Our results demonstrate that hydrothermal fluid–rock interactions can rapidly shift shallow volcanic faults across slip modes by modifying fault fabric, stiffness, and strength. Temperature-driven mineral breakdown and pore-space sealing play a fundamental but often overlooked role in the shallow seismicity at Campi Flegrei, as well as in similar tuffaceous geothermal reservoirs, with important implications for fault mechanics, seismic hazard, and volcanic dynamics across small-to-long term time scales.

How to cite: D'Ippolito, G., Tesei, T., Mormone, A., Gomila, R., Piochi, M., and Di Toro, G.: Seismicity driven by rapid fault cementation in tuffs under hydrothermal conditions of the Campi Flegrei caldera (Italy), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6931, https://doi.org/10.5194/egusphere-egu26-6931, 2026.

EGU26-7648 | ECS | Posters on site | TS3.3

Aseismic slip along the evaporite-rich Katouna-Stamna fault in Greece 

Silvia Crosetto, Joel Szrek, Sabrina Metzger, Giorgio Gomba, Claudio Faccenna, and Romain Jolivet

The left-lateral, NW-trending Katouna–Stamna Fault (KSF) in Western Greece marks the NE-boundary of the Ionian-Akarnania block. The Global Navigation Satellite System (GNSS) displacement field suggest the potential presence of aseismic slip, which is corroborated by the minimal seismicity in the area. To better understand the current kinematics of the KSF, we integrate full-coverage surface displacement rates derived from 7-yr-long Interferometric Synthetic-Aperture Radar (InSAR) time-series with the GNSS rates, field observations, and structural analyses.

While previous geodetic studies suggested a strike-slip rate of ∼10 mm/yr, our distributed-slip model indicates a strike-slip rate of up to 19 ± 1 mm/yr and a dip-slip rate of up to 11 ± 7 mm/yr. In particular, sinistral slip localises in the right-stepping south-central fault segment, while the highest dip-slip value is found in the northwestern part. In the model, aseismic slip reaches the surface, but the highest slip rates are found below 5 km depth. Furthermore, only the northernmost part of the fault appears locked and accumulating elastic strain, which also corresponds to the location of an earthquake occurred in 2014, supporting our model.

Field evidence indicates complex fault kinematics with multiple deformation phases. The younger generation of NNW-trending striae shows mostly oblique motion with dominating strike-slip component, in agreement with geodetic observations. Such agreement indicates that the geological kinematic regime under which they formed may be relatively recent and possibly still in place.

Overall, our geological observations highlight several possible drivers of aseismic slip. The fault bounds a so-called ‘salt wall’, represented by an elongated evaporite – mainly gypsum – diapir intruding the carbonate bedrock. Although dry gypsum does not display aseismic behaviour on its own, the interaction between evaporites and fluids could promote pressure-solution creep in wet gypsum. Pressure-solution creep in the fault gouge has been reported for other creeping faults, namely the San Andreas Fault, the North Anatolian Fault and the Longitudinal Valley Fault.

Structural evidence of ductile shear deformation within the evaporite-bearing rock along the KSF suggests that, at least in the shallow part, slip may occur with predominantly ductile creeping. This process is facilitated by the high solubility of evaporites and by the presence of fluids, and could explain both ductile deformation and abundant veining observed on the field. Furthermore, the fact that pressure-solution is slower between identical minerals, due to healed boundaries, but faster between different minerals, notably halite and calcite, would explain why the deformation is localised along the contact between evaporites and carbonates, possibly on both sides of the salt wall.

How to cite: Crosetto, S., Szrek, J., Metzger, S., Gomba, G., Faccenna, C., and Jolivet, R.: Aseismic slip along the evaporite-rich Katouna-Stamna fault in Greece, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7648, https://doi.org/10.5194/egusphere-egu26-7648, 2026.

EGU26-8288 | ECS | Posters on site | TS3.3

From seismic to aseismic slip in the lower crust: Results from hydrothermal ring-shear experiments 

Lawrencia Mensah, André R. Niemeijer, Marco Herwegh, and Alfons Berger

Understanding why earthquakes nucleate unusually deep in the crust is essential for improving seismic hazard assessments. These events occur under pressures and temperatures where rocks are expected to deform ductilely, challenging standard models of rock strength and faulting. Constraining the conditions that allow frictional instabilities to persist at depth therefore has important scientific and societal implications. To investigate the transition from potentially seismic to aseismic slip in lower-crustal environments, we conducted hydrothermal friction experiments on simulated gouges derived from epidote-rich (65%) and amphibole-rich (58%) basement gneiss from the western branch of the East African Rift System. We characterized their frictional strength and stability across temperatures of 350-600 °C, 150 MPa effective normal stress, and 100 MPa pore fluid pressure. We tested three slip-velocity protocols spanning slow (0.01-1 μm/s), intermediate (0.1-10 μm/s), and fast (1-100 μm/s) rates. Both samples show frictional strengths that vary with temperature and slip velocity. Rate-and-state friction parameters (a-b) indicate that the epidote-rich gouge exhibits velocity-weakening behaviour between 350-500 °C and at 0.3-100 μm/s, whereas the amphibole-rich gouge remains velocity-weakening across the full temperature range and at 1-100 μm/s. Microstructural observations indicate that deformation is primarily accommodated within a broad slip zone, where frictional granular flow and cataclasis dominate under both high- and low-temperature conditions. At the highest temperatures (600 °C) and slow slip rates, however, additional evidence for dissolution-precipitation creep was found, indicating the operation of viscous deformation. Our results suggest that epidote and amphibole-rich gouges can host seismic slip under lower-crustal temperature conditions at elevated slip rates. Under natural lower-crustal conditions, these elevated slip rates, sufficient to trigger frictional instability, could be facilitated temporarily by stress transfer, strain localization, or transient fluid-pressure variations.

How to cite: Mensah, L., Niemeijer, A. R., Herwegh, M., and Berger, A.: From seismic to aseismic slip in the lower crust: Results from hydrothermal ring-shear experiments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8288, https://doi.org/10.5194/egusphere-egu26-8288, 2026.

EGU26-9011 | ECS | Posters on site | TS3.3

Dominant Control of 3D Fault Geometry on the Seismogenic Environment of the Longmenshan Fault: Insights from Multi-Source Data-Constrained 3D Numerical Modeling of the Eastern Tibetan Plateau 

Yixuan Yang, Wei Tao, Junxiang Qiao, Haoyue Sun, Xuhang Yang, Renqi Lu, Wei Wang, Xiao Sun, Fang Xu, and Xin Wang

In this study, we constructed a 3D viscoelastic finite element model of the lithosphere in the eastern Tibetan Plateau, incorporating fine-scale 3D fault geometries rigorously constrained by multi-source data. We quantitatively analyzed the seismogenic mechanisms and controlling factors of the Longmenshan Fault Zone (LMSFZ). The results indicate that: (1) Regional deformation is co-governed by the synergistic mechanism of "rigid blocking by the Sichuan Basin" and "kinematic decoupling along major strike-slip faults." (2) The 3D fault geometry serves as the primary factor controlling stress accumulation on the LMSFZ, following a physical control chain of "Geometry → Mechanical Response → Kinematic Characteristics." Vertically, the listric geometry results in a stratified feature of "deep-driving and shallow-locking"; along the strike, geometric variations dominate the mode transition from "thrust-strike-slip coupling" to "strike-slip dominance." (3) Seismic hazard assessment identifies a high-risk "unruptured asperity" near Dachuan in the southwestern segment, where the deep strain energy density is comparable to that of the Wenchuan earthquake nucleation zone. Conversely, the northeastern segment is characterized by a "low-resistance/slip-deficit" mode, indicating high long-term seismic hazard. Based on physically self-consistent heterogeneous continuum mechanical modeling, this study transcends the limitations of discrete surface observations. It achieves a transition from 2D surface projections to deep 3D continuous fields, providing a reliable physical basis for quantitatively unraveling the deep seismogenic mechanisms of faults.

How to cite: Yang, Y., Tao, W., Qiao, J., Sun, H., Yang, X., Lu, R., Wang, W., Sun, X., Xu, F., and Wang, X.: Dominant Control of 3D Fault Geometry on the Seismogenic Environment of the Longmenshan Fault: Insights from Multi-Source Data-Constrained 3D Numerical Modeling of the Eastern Tibetan Plateau, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9011, https://doi.org/10.5194/egusphere-egu26-9011, 2026.

EGU26-9321 | Posters on site | TS3.3

Mixed mode of deformation and processes along the Tellaro Detachment (Northern Apennines, Italy) 

Giancarlo Molli, Luigi Berio, Mattia Pizzati, Alessio Lucca, Pensiero Cecchini, Fabrizio Balsamo, and Fabrizio Storti

In the inner Northern Apennines (Lerici and La Spezia inland) the exhumed Tellaro detachment fault system is exposed. It can be traced in an area larger than 20 Km2 and well observable in continuous kilometer-long coast exposures (Storti, 1995; Clemenzi et al., 2015). The major low-angle fault zone is marked by decameter-thick, carbonate-rich, cataclasites and gouges (“Calcare Cavernoso Fm.”) overlying a footwall of cataclastically deformed low-grade quarzites, phyllites and metaconglomerates (Ladinian-Carnian Verrucano Fm.) belonging to the Tuscan Metamorphic units (Molli et al., 2018). In the hanging wall, synthetic and antithetic splay faults affect the originally ~6 Km-thick Tuscan Nappe succession, thinned to less than 0.6 Km.

Detailed structural data collected at the meso- and microscale, combined with Raman spectroscopy, fluid-inclusion analysis, and mineralogical studies, allowed us to constraints deformation processes and fault activity in a temperature range of 260-120 °C at mid-shallow crustal depth (10-5 Km). Observable deformation structures in the footwall fault rocks provide evidence supporting mixed deformation mode and mechanisms, with intermitted cataclastic flow and unstable brittle slip (aseismic-to-seismic) during the fault activity.

How to cite: Molli, G., Berio, L., Pizzati, M., Lucca, A., Cecchini, P., Balsamo, F., and Storti, F.: Mixed mode of deformation and processes along the Tellaro Detachment (Northern Apennines, Italy), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9321, https://doi.org/10.5194/egusphere-egu26-9321, 2026.

Serpentinites are “weak" rocks common in several geodynamics settings, including mid-ocean ridges, transform faults and subduction zones. Because of this, serpentinites play a pivotal role in the nucleation and propagation of slow and regular earthquakes.

We studied serpentinites pertaining to the exhumed Monte Fico shear zone (Elba Island, Italy) that reached greenschist facies conditions during deformation. The shear zone, tens to hundreds of m thick, is made of 10-100 cm lenses of metaperidotite, mainly composed by the lizardite and chrysotile, wrapped by foliated serpentinites. Bulk deformation is accommodated by anastomosing and pervasive S/C foliations. The lenses are bounded by 1-3 cm thick brittle faults decorated by slickenfibers composed of chrysotile and polygonal serpentine.

To determine the frictional and healing properties of the serpentinite-bearing shear zones and faults under realistic ambient shallow-subduction conditions, we performed 39 slide-hold-slide experiments at σ’n=20 MPa, Pf=6 MPa, Vshear= 10 µm/s and at temperatures from 25°C to 400°C. We sheared with a rotary shear apparatus equipped with a hydrothermal vessel (ROSA-HYDROS, Dept. of Geosciences, UniPD, Italy) the powders obtained from the metaperidotite and the slickenfibers.

Regarding the frictional properties of the metaperidotite, when the water is in a liquid state, the friction coefficient increases from 0.3 at 25°C to 0.5 at 300°C; when water is in vapour and supercritical states, the friction coefficient is strain hardening (0.6-0.89 at 300°C-400°C). Stick-slip behaviour (i.e., seismic slip) is observed only at 400°C. In the case of slickenfibers, when the water is in liquid state, the friction coefficient increases from 0.23 at 25°C to 0.34 at 300°C. When water is in vapour conditions the friction coefficient is 0.47 at 300°C and 0.57 at 400°C. In conclusion, the metaperidotite can deform by aseismic creep or seismic slip and the slickenfibers deform by aseismic creep.

Regarding the frictional healing properties, it differs between metaperidotite and slickenfibers. Frictional healing of the metaperidotite is positive and increases with temperature, independently of the physical state of water. Instead, frictional healing of the slickenfibers is negative for nearly all the conditions, with a maximum positive healing between 150°C and 250°C.

Our results show that the frictional response of low-grade serpentinites sheared in the laboratory at shallow-subduction hydrothermal conditions is controlled by the mineral assemblage and temperature. As a consequence, in nature, the combination of frictional and healing behaviour is highly heterogeneous and becomes the driver for enhanced instabilities on the weak but fast-healing slickenfibers in a narrow temperature window between 150°C and 250°C.

How to cite: Salvadori, L., Di Toro, G., and Tesei, T.: Temperature-dependent frictional and healing behaviour in serpentinite shear zones: implications for subduction zone seismicity, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9588, https://doi.org/10.5194/egusphere-egu26-9588, 2026.

EGU26-10168 | Posters on site | TS3.3

Strain hardening as a mechanism for slip nucleation and arrest in phyllosilicate-rich rocks 

Telemaco Tesei, Leonardo Salvadori, Giulio Di Toro, and André Niemeijer

The processes governing the nucleation and arrest of a rupture during slow slips remain speculative. The importance of understanding slip arrest mechanisms lies in the potential for slow slips to trigger destructive earthquakes and in the fact that not all slow slips lead to the nucleation of regular earthquakes.

At seismogenic depths (<30 Km, 100°-400°C), phyllosilicate-rich rocks (i.e., claystones, metasediments, serpentinites) are widespread lithologies that are also frictionally weak (µ≪0.6). The presence of these rock favors slip nucleation at weak fault patches which may or may not develop into fast unstable slip.

We performed hydrothermal friction experiments at the temperatures and pressures relevant to the seismogenic zone to understand the mechanism(s) behind slip nucleation and arrest. We tested experimental gouges of phyllite (Rio Marina Fm.) and meta-sandstone (Verrucano Fm.) from a natural shear zone exposed at the Elba Island (Italy). Experiments were performed at a shearing velocity of 10 µm/s over a wide range of effective normal stresses (20 to 150 MPa), high temperature (350 °C) conditions and to high strains (displacements up to 40 mm) using two hydrothermal Rotary shear machines hosted in Padova University (Italy) and Utrecht University (Netherlands).

            Experimental results show that the phyllite sheared at low effective normal stresses (20-50 MPa), show a low friction coefficient of µ ~ 0.3 and a strain weakening behavior. With increasing normal stress (up to 150 MPa) we observe an initial low friction (0.35) that evolves with a strain hardening trend up to µ ~ 0.7-0.9. Conversely, experiments on the meta-sandstone show generally higher friction (0.6-0.7) even at small strains at all normal stress conditions.

Frictional weakness is due to the phyllosilicates’ ability to develop efficient foliations that accommodate the deformation. At low effective normal stresses (up to 60 MPa), we observe the development of a through-going phyllosilicate network within the phyllite gouge resulting in the observed low friction and strain weakening evolution. Conversely, at high normal stress, a through-going weak phyllosilicate network cannot develop because of the presence of frictionally strong high stress asperities, from which phyllosilicates have been extruded. The observed strain hardening and high friction trend results from comminution of intervening quartz and feldspar grains that we correlate with the occurrence of ultracataclasites in the microstructures. The experimental results on the meta-sandstone confirm this hypothesis, showing a friction and a microstructure similar to the “hardened” phyllite gouges. EDS maps of chemical elements in the phyllite gouge sheared under high normal stress confirm the absence of an interconnected network of phyllosilicates. In natural shear zones, at seismogenic depth, we may observe slip nucleation in weak phyllosilicate rich rocks (µ ~ 0.3). However, the fault patch may quickly strengthen if the propagating slip is fast enough to disrupt the foliation, which would decelerate slip. Our study provides a new mechanism by which slow slip events may nucleate and spontaneously arrest, potentially halting the growth of rupture into regular earthquakes.

How to cite: Tesei, T., Salvadori, L., Di Toro, G., and Niemeijer, A.: Strain hardening as a mechanism for slip nucleation and arrest in phyllosilicate-rich rocks, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10168, https://doi.org/10.5194/egusphere-egu26-10168, 2026.

EGU26-11504 | Posters on site | TS3.3

3D Structural Characterization and Analogue Modeling to Constrain the growth and evolution of the Yusuf Fault (Alborán Sea) 

Hector Perea, Nathalia Mattos, Oriol Ferrer, Oscar Gratacós, Eloi Carola, Ariadna Canari, and Sara Martíniez-Loriente

The Yusuf Fault system (YF) is one of the largest active strike-slip structures in the Alborán Sea, where it acts as a lithospheric-scale boundary accommodating part of the NW-SE convergence between the Nubian and Eurasian plates. It trends WNW-ESE, extends for ~150 km, and is characterized by a complex fault array and a prominent pull-apart basin. Accurate representation of its 3D geometry and seismogenic behavior is essential to constrain its seismic potential and understand the tectonic evolution of the region. In this study, we integrate multibeam bathymetry, high-resolution multi-channel seismic reflection (HR-MCS) data, and scaled analogue modeling to characterize the structural architecture and kinematic evolution of the YF. Bathymetric analysis using topographic attributes enabled detailed mapping of the fault trace and associated geomorphic features, while seismic data interpretation revealed subsurface discontinuities and fault offsets affecting key seismostratigraphic units from the Upper Miocene to the Quaternary. This information allowed us to construct the first 3D structural model of the YF, showing that the system consists of multiple overlapping segments forming a complex strike-slip fault architecture. To explore the processes controlling pull-apart basin development, we conducted analogue experiments simulating strike-slip fault interaction. Results suggest that basin opening is controlled by overlapped fault geometry and lateral displacement rates, providing a physical framework for interpreting the observed morphostructural patterns. This integrated approach improves constraints on fault growth and segmentation, offering critical input for seismic hazard models in the western Mediterranean.

How to cite: Perea, H., Mattos, N., Ferrer, O., Gratacós, O., Carola, E., Canari, A., and Martíniez-Loriente, S.: 3D Structural Characterization and Analogue Modeling to Constrain the growth and evolution of the Yusuf Fault (Alborán Sea), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11504, https://doi.org/10.5194/egusphere-egu26-11504, 2026.

EGU26-13810 | ECS | Orals | TS3.3

Post-earthquake Fault Zone Overstrengthening Influences Slip during Future Earthquakes 

Zachary Smith, Roland Bürgmann, Francis Waligora, Ashley Griffith, Johanna Nevitt, Kathryn Materna, Matthew Gleeson, Ruyu Yan, and Matthew Idzakovich

Changes in fault-zone properties over successive earthquake cycles drive variations in fault slip behavior and seismic hazard. Typically, fault zones are believed to evolve towards tabular damage zones surrounding a low cohesion fault core and are characterized by increased fracture density and reduced elastic stiffness. However, interseismic mineral alteration and fracture healing can either weaken or strengthen fault zones, influencing future earthquake ruptures. Here, we document post-earthquake fault-zone-strength enhancement through field and laboratory observations of fault core and damage zone rocks from subsidiary faults partially activated during the 2019 Ridgecrest earthquake sequence. Analysis of coseismic slip observed with InSAR shows that only some portions of faults in the Spangler Hills experienced slip during the Ridgecrest earthquake sequence even though Coulomb failure stress change analysis predicts the entire length of the faults would have been stressed towards failure. Field investigations have revealed the presence of pseudotachylyte along the faults which is evidence of ancient earthquakes. Mineralogical analysis of healed pulverized rock within these fault zones suggests that these early earthquakes occurred near the brittle-ductile transition prior to exhumation. We measured the tensile and uniaxial compressive strength, Young's modulus, Poisson's Ratio, cohesion, and angle of internal friction of exhumed fault zone rocks and nearby plutonic rocks using a Split Hopkinson Pressure Bar. We find that post-earthquake healing via propylitic albitic alteration within the fault zone increased damage zone tensile and compressive strength and stiffness, and fault core cohesion by ~150% in the location where no slip was observed. These observations are further supported by multispectral Landsat and ASTER analyses, which indicate that surface slip along subsidiary faults is preferentially localized within zones of pre-existing phyllic hydrothermal alteration and terminates at the boundaries of propylitic alteration zones. Together, these results demonstrate that fault-zone cohesive healing can exert long-lasting control on fault slip behavior and seismic hazards.

How to cite: Smith, Z., Bürgmann, R., Waligora, F., Griffith, A., Nevitt, J., Materna, K., Gleeson, M., Yan, R., and Idzakovich, M.: Post-earthquake Fault Zone Overstrengthening Influences Slip during Future Earthquakes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13810, https://doi.org/10.5194/egusphere-egu26-13810, 2026.

EGU26-13844 | ECS | Posters on site | TS3.3

Tracing fluid sources, their influence, and mechanical consequences in the Inuyama accretionary complex, Japan 

Rebecca V M Robertson, Giovanni Toffol, Ake Fagereng, Kohtaro Ujiie, and Joaquin Julve

Vein stable isotope geochemistry and minerology provide a powerful record of fluid sources in subduction-zone fault systems, with implications for fault mechanics and seismic behaviour. We investigate fluid sources along out-of-sequence thrusts within an exceptionally well-preserved exhumed analogue of the shallow seismogenic zone: the Inuyama Sequence from the Jurassic Accretionary Complex in central Japan. The sequence comprises a coherent ocean-floor stratigraphy of siliceous claystone, ribbon chert, siliceous mudstone and clastic units, repeated by thrust imbrication.

Vein and host rock stable isotope data reveal the presence of two distinct vein sets, implying two distinct fluids, within the thrust sheets. One fluid is a cool pore water (𝛿18O = - 4 to 0 ‰), that precipitated quartz (21.2 to 25.7 ‰), calcite (20.6 to 21.1 ‰), and rhodochrosite (25.2 ‰) veins at ∼40 to100 ˚C throughout the exposed thrust sheets. This is consistent with a seawater-derived pore fluid in the shallow accretionary prism. In contrast, some quartz (2.1 ‰) and calcite (-0.4 to 6.2 ‰) vein clusters require a different and warmer fluid (𝛿18O = - 11 to - 8 ‰) possibly of meteoric origin. These isotopically lighter veins are restricted to discrete shear zones with well-developed scaly fabric and are generally focused along the margins of mechanically competent blocks. Notably, these discrete shear zones have far higher carbon contents than the host rocks, be that through pressure solution or direct carbon precipitation. The isotopically lighter calcite and quartz veins record significantly higher temperatures (∼170 to 220 ˚C), confirmed with chlorite geothermometry, and are in line with Raman and vitrinite reflectance temperature estimates for peak conditions for the area (Kameda et al., 2012; Ujiie et al., 2021).

The occurrence of isotopically light fluids at temperatures of 170-220˚C, corresponding to depths of ~ 8.5 to11 km given a relatively cool accretionary geotherm (20 ˚C/km), requires either (1) deep and lateral ingress of meteoric waters into the inner wedge as accreted sediments approached the coast, (2) late-stage vein precipitation during exhumation and fault reactivation, or (3) kinetic isotope effects associated with rapid precipitation during fault dilation that drives 𝛿18O lower than those predicted for equilibrium precipitation. Importantly, the hot and isotopically light fluids show a strong spatial relationship with highly concentrated black carbonaceous material that appears to control strain localisation at thrust sheet contacts. Consequently, these fluid-driven mechanical changes may have created carbon-rich asperities of very low frictional strength, encouraging local aseismic creep and stress build up at asperity boundaries.

How to cite: Robertson, R. V. M., Toffol, G., Fagereng, A., Ujiie, K., and Julve, J.: Tracing fluid sources, their influence, and mechanical consequences in the Inuyama accretionary complex, Japan, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13844, https://doi.org/10.5194/egusphere-egu26-13844, 2026.

EGU26-14249 | Orals | TS3.3

Signatures of changing deformation rate dynamics in deforming rocks: Examples from the exhumed Slow Earthquake Zone of New Caledonia 

Sandra Piazolo, Manon Carpenter, Timothy Chapman, Geoffrey Clarke, Lars Hansen, and Jessica Hawthorne

Deformation on planetary bodies is characterized by processes that act at strain rates of more than 15 orders of magnitude difference. With the advent of advanced geophysical techniques with ever increasing resolution in time and space, we are now able to detect some of these intriguing dynamics. However, to improve earthquake related hazard assessments, advancing from observations of apparent dynamics of geophysically detected deformation events to in-depth understanding of the underlying physical processes is urgently needed. One “type” example of a deformation phenomenon encompassing deformation at different rates are Slow Earthquakes (SEs). In SEs, slip occurs more slowly than in regular earthquakes, but significantly faster than can be attributed to long-term plate motion. Although SEs are abundant, their geophysically observed characteristics cannot be reconciled with current understanding of how rocks deform: new evidence of slip processes need to be discovered in the geological record.
         Rock outcrops from an example of exhumed subducted crust in New Caledonia are interpreted to contain zones of former SEs. Microstructural characterization combining EBSD and EDS analyses deciphers controlling deformation processes, while phase petrology is used to evaluate stages of fluid ingress, production or egress. Based on our observations, we interpret that several deformation processes directly associated with the presence and movement of fluids governed rock behaviour. Relatively “slow” dissolution-precipitation creep is the main “background” deformation process responsible for the observed shape- and crystallographic-preferred orientations, in-grain compositional variations and grain boundary alignment. Geometric features akin to soft sediment deformation structures and water escape structures that developed at high grade conditions suggest that intermittently, local liquefaction is triggered by episodic high fluid pressures induced by mineral dehydration reactions. Based on these observations, we propose that wet granular flow at high fluid pressure may occur in subduction zone environments. This process is transient and relatively fast contrasting the slow, continuous viscous background flow. Catastrophic failure and flow by wet granular flow represents a viable candidate process for geophysically observed transient high slip rates in fluid rich subduction environments.

How to cite: Piazolo, S., Carpenter, M., Chapman, T., Clarke, G., Hansen, L., and Hawthorne, J.: Signatures of changing deformation rate dynamics in deforming rocks: Examples from the exhumed Slow Earthquake Zone of New Caledonia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14249, https://doi.org/10.5194/egusphere-egu26-14249, 2026.

EGU26-14779 | ECS | Posters on site | TS3.3

Fault contact evolution seen via total internal reflection and heard via acoustic emissions 

Charlotte Bate, Christine McCarthy, Will Steinhardt, and Seth Saltiel

Earthquakes and ice sheet collapse are significant hazards that are both governed by friction. Fault interfaces and glacier beds share many frictional behaviours: slip stability and instability, seismicity, healing, and episodic slip. Rate-and-state friction (RSF), an empirically derived framework for describing frictional strength, has been successfully utilized for the last five decades to quantitatively characterize earthquake phenomena and has more recently been employed to describe stick-slip behaviour of glaciers. While RSF has been used to extract consistent parameters in both systems, frictional behaviours are rooted in the evolution of the asperities in contact at the interface. Although RSF is powerful (and practical!), it does not reveal the micromechanisms driving the behaviour it describes, nor does it account for other behaviours, such as rupture initiation and variation in stress drop. For this reason, we take advantage of the transparency of ice, its faster deformation timescales, as well as the frictional properties ice shares with rock, to directly observe the frictional interface in situ during shear. To do this, we employ a novel adaptation to our cryogenic biaxial device. As the interface cycles between periods of holds and shears, we use 1) an optical technique, total internal reflection, to light up the interface contacts and observe their evolution, and 2) acoustic emission sensors to listen to and locate slip events. This unique combination of data will allow us to more comprehensively understand the contact-level mechanisms that control friction on deforming interfaces, and help us to better interpret the seismological data we measure on faults and ice sheets. Here, we present recent results of this work.

How to cite: Bate, C., McCarthy, C., Steinhardt, W., and Saltiel, S.: Fault contact evolution seen via total internal reflection and heard via acoustic emissions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14779, https://doi.org/10.5194/egusphere-egu26-14779, 2026.

This study presents an analysis of the tectonic evolution and structural features of west-central Taiwan, focusing on the fold-and-thrust belt developed from the Late Miocene–Holocene. Integrating surface geological mapping, borehole data, and seismic reflection profiles, we establish a refined tectonic model that emphasizes the significant influence of the preexisting normal fault on structural development. Our findings demonstrate that pronounced variations in stratigraphic thickness, notably within the early foreland basin sequence, indicate syndepositional normal faulting, creating substantial accommodation space during sedimentation. The normal fault acted as a mechanical barrier was overstepped by a thrust ramp during later compressional phases. These inherited structural features significantly influence seismicity and deformation patterns, exemplified by mechanical barriers linked to the 1999 Chi-Chi earthquake. Our structural cross sections reveal a characteristic ramp-flat-ramp geometry linked to the Changhua Thrust, the Chelungpu Thrust, and the Chusiang Fault. The resulting structural model illustrates a sequential tectonic evolution, transitioning from early extensional regimes to complex compressional environments.

How to cite: Chang, C.-W., Huang, W.-J., and Huang, T.-C.: Preexisting Normal Fault with Pliocene Syndepositional Controls on the Structural Style Transition: Implications for the Structural Evolution in Thrust Belts, West-Central Taiwan, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15085, https://doi.org/10.5194/egusphere-egu26-15085, 2026.

EGU26-15670 | ECS | Posters on site | TS3.3

Possible cascading ruptures on the eastern section of the Altyn Tagh fault 

Yanxiu Shao, Jerome van der Woerd, Jing Liu-Zeng, Boming Li, and Shihao Zhang

Understanding how connected fault segments may rupture sequentially or simultaneously to produce large earthquakes is a fundamental problem in earthquake physics and seismic hazard assessment. Addressing this issue requires integrated constraints on fault geometry, slip behavior, and rupture history across interconnected fault systems. The Subei triple junction along the eastern section of the Altyn Tagh fault, which connects thrust (Danghe Nan Shan thrust) and strike-slip fault segments (Altyn Tagh and Yema-Daxue Shan faults), is an ideal site for investigating such cascading rupture processes. In this study, we excavated three new paleoseismic trenches around the Subei junction, including two across the Danghe Nan Shan thrust and one across the Altyn Tagh fault. Detailed stratigraphic logging, identification of abundant paleoseismic indicators, and dense optical stimulated luminescence (OSL) dating constrain the timing of late Quaternary surface-rupturing earthquakes. Our results indicate that three to four surface-rupturing events occurred at these sites during the Holocene, with overlapping age ranges among the different fault segments. By integrating our new paleoseismic constraints with previously studies, we identify at least one Holocene earthquake that likely involved synchronous rupture of the Altyn Tagh fault, the Yema–Daxue Shan fault, and the Danghe Nan Shan thrust. Multicycle dynamic rupture modeling incorporating fault geometry and long-term slip rates further support such cascading ruptures across the strike-slip and thrust fault network. These results provide rare field-based evidence that large earthquakes on the eastern section of Altyn Tagh fault may involve multiple fault segment ruptures. Our findings highlight the importance of considering fault interactions and cascading rupture scenarios when assessing seismic hazard in complex continental fault systems.

How to cite: Shao, Y., van der Woerd, J., Liu-Zeng, J., Li, B., and Zhang, S.: Possible cascading ruptures on the eastern section of the Altyn Tagh fault, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15670, https://doi.org/10.5194/egusphere-egu26-15670, 2026.

Abstract: The collision and compression between the Indian and Eurasian plates have resulted in intense crustal shortening and deformation in the Tian Shan since the Cenozoic, leading to its renewed uplift and making the Tian Shan one of the most intensely deformed intracontinental orogenic belts and seismically active regions in the world. Cenozoic deformation of the Tian Shan is characterized by north–south crustal shortening, which is mainly controlled by approximately E-W striking thrust faults, N-W striking dextral strike-slip faults, and N-E striking sinistral strike-slip faults. Concurrently, pronounced tectonic deformation occurred within the Tien Shan, forming a series of E-W trending intermontane basins, including the Turpan, Kumishi, Yanqi, and Yili basins. The Yanqi Basin, located in the southeastern Tian Shan, has experienced significant tectonic deformation due to the continuous uplift of the Tien Shan. Since the Late Quaternary, tectonic deformation has been mainly concentrated along the northern and southern margins of the basin. Two major active tectonic systems are developed along the northern margin, including the Yanqi Basin north-edge thrust fault and the piedmont thrust-fold belt. Along the southern margin, the Yanqi Basin south-edge thrust fault is developed, striking E-W and dipping southward, forming a complex thrust-fold belt. Within this fold belt on the southern margin of the basin, Quaternary geomorphic surfaces are well preserved and display fault scarps of variable heights. Multiple generations of alluvial fans are dissected along the fault scarps. In this study, high-resolution topographic data of faulted alluvial fan landforms along the southern margin thrust-fold belt were acquired using airborne LiDAR. Detailed geomorphic interpretation and quantitative analysis were conducted to identify multiple generations of landforms developed perpendicular to the fault strike. Based on comprehensive geomorphic interpretation and field investigations, deposits from different generations of alluvial fans were sampled for surface age determination. Furthermore, based on measurements of exposed strata and the construction of characteristic topographic profiles across the alluvial fans, we established the cross-sectional geometry and deformation model of the thrust fault-fold belt at the south-edge of the Yanqi Basin. By integrating the tri-shear fault-propagation fold model from fault-related fold theory, we constrain the shortening deformation characteristics of the thrust fault-fold belt.  This allows us to estimate the shortening amount and shortening rate for the belt at the southern margin of the Yanqi Basin.  Combined with analysis of surrounding fold deformation and fault slip rates, this work not only reveals the deep geometry and activity mechanism of the thrust fault at the south-edge of the Yanqi Basin but also provides constraints for understanding intracontinental deformation within the Southern Tian Shan.

How to cite: Yang, J., Zheng, W., and Zhang, D.: Quantitative constraints on shortening deformation characteristics of the fold at the south-edge thrust fault of the Yanqi Basin, Southern Tien Shan , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15676, https://doi.org/10.5194/egusphere-egu26-15676, 2026.

EGU26-16525 | ECS | Posters on site | TS3.3

Lithologic Controls on Frictional Behavior Along the Shallow Subduction Interface: Constraints From an Exhumed Accretionary Wedge (McHugh Complex, Alaska) 

Markus Rast, Whitney Behr, Claudio Madonna, and Simon Guérin-Marthe

Subduction zone megathrusts accommodate a wide range of slip modes, from earthquakes to slow slip events (SSEs) and aseismic creep. Understanding why different slip modes localize in specific regions of the shallow subduction interface remains a significant challenge. Exhumed accretionary complexes are an important natural laboratory for addressing this problem. In this study, we examine the mechanical behavior of representative lithologies and faults within the McHugh Complex in the Kenai Mountains of southern Alaska. The McHugh Complex is a Mesozoic accretionary wedge that exposes lithologies and fault zones representative of the shallow subduction interface. We integrate field observations with compositional and microstructural analyses and laboratory friction experiments to evaluate both fault failure conditions and potential slip modes. Direct shear experiments were conducted on powdered fault gouges and host rocks under dry and water-saturated conditions at normal stresses of 10–40 MPa, representative of shallow subduction zone conditions. 
Our results demonstrate that mineralogical composition exerts a first-order control on fault strength and frictional stability. Increasing proportions of phyllosilicates reduce friction coefficients (μf) and promote velocity-strengthening behavior. Argillitic fault gouges rich in organic matter exhibit the lowest frictional strength (μf = 0.33), consistent with strain localization observed in these rocks in the field. Conversely, stronger lithologies, such as pillow basalts and cherts, display higher frictional strengths (μf = 0.53) and frictional stabilities that promote seismic slip initiation. However, fault zones within basaltic units that have undergone significant alteration and chlorite enrichment evolve toward velocity-neutral behavior, suggesting the potential to nucleate SSEs rather than earthquakes. 
A cross-section through the exhumed accretionary wedge reveals that contrasts in mechanical strength often coincide with contrasts in permeability, suggesting that stress concentrations and transient fluid overpressure likely act together to trigger fault failure. Overall, our findings emphasize the role of lithologic heterogeneity in controlling both fault failure and slip mode along the shallow subduction interface. This provides a framework for linking rock composition to the spatial distribution of seismic and aseismic behavior. Future work will apply this integrated approach to additional cross-sections across the McHugh Complex.

How to cite: Rast, M., Behr, W., Madonna, C., and Guérin-Marthe, S.: Lithologic Controls on Frictional Behavior Along the Shallow Subduction Interface: Constraints From an Exhumed Accretionary Wedge (McHugh Complex, Alaska), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16525, https://doi.org/10.5194/egusphere-egu26-16525, 2026.

EGU26-16986 | Posters on site | TS3.3

The Subei triple junction: a complex strike-slip – thrust junction allowing strain transfer from the Altyn-Tagh fault to the Qilian Shan  

Jerome van der Woerd, Yanxiu Shao, Daohuang Yuan, and Jing Liu-Zeng

Slip-rate decrease along the eastern Altyn Tagh fault has long been interpreted as due to strain transfer from the strike-slip fault to the sequential thrust splays of the Qilian Shan. While the 2D kinematics of such strain transfer is now becoming well documented thanks to numerous field studies as well as an increase in geodetic and InSAR data, how the structures connect, interact during large rupturing events and evolve on the long-term is not well known. We focus on the Danghe Nan Shan thrust, a major splay of the Altyn Tagh fault (ATF), at one of these complex fault junctions. Near Subei, the western Danghe Nan Shan thrust comprises two left-stepping faults outlined by fault scarps in front of folded and uplifted alluvial fans and terraces. Age constraints of the accumulated slip of four terraces standing 7–60 m above the present stream bed yield shortening and vertical uplift rates of 0.5 ± 0.1 and 1.1 ± 0.3 mm/yr, respectively, over the last 130 ka on one of the thrust. Overall, about 1-1.4 mm/yr uplift and shortening rates are determined, in agreement with late Miocene long-term exhumation rate estimates. We emphasize the need for precise long-term slip rate determination and understanding the three-dimensional structures of fault connections to evaluate strain transfer between faults and related seismic hazard on these complex fault systems.

How to cite: van der Woerd, J., Shao, Y., Yuan, D., and Liu-Zeng, J.: The Subei triple junction: a complex strike-slip – thrust junction allowing strain transfer from the Altyn-Tagh fault to the Qilian Shan , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16986, https://doi.org/10.5194/egusphere-egu26-16986, 2026.

EGU26-17287 | ECS | Posters on site | TS3.3

Accretionary complex heterogeneity controls the faulting style of upper plate thrusts 

Giovanni Toffol, Rebecca V M Robertson, Åke Fagereng, Kohtaro Ujiie, and Joaquin Julve Lillo

A relevant portion of seismic activity in subduction zones takes place along splay faults and other subsidiary structures of the subduction interface that cut across the upper plate accretionary complex. The heterogeneous lithology of accretionary complexes, reflecting the stratigraphy of the incoming ocean plate, exerts a first-order control on the seismic behaviour. Thus, investigating accretionary complexes exhumed from the seismogenic zone is relevant to understand upper plate seismicity.

The Inuyama Sequence, part of the Jurassic Accretionary Complex of central Japan, is the ideal natural laboratory to investigate the lithological control on faulting style and seismic/aseismic behaviour in the shallow, sediment-dominated portion of an accretionary prism. It consists of a coherent chert-clastic complex with ocean-floor stratigraphy (in ascending order: siliceous claystone unit, ribbon chert unit, siliceous mudstone unit, and a clastic unit composed of lower mudstone, sandstone and upper mudstone) repeated six times by out-of-sequence thrusts that delimit the thrusts sheets [1].

Here we focus on three of the out-of-sequence thrusts (T1, T2, T3 in ascending structural order) that are well exposed along the Kiso River: T1 separates siliceous mudstones of sheet 1 from black and grey cherts of sheet 2; T2 separates upper mudstones of sheet 2 from siliceous claystones and cherts of sheet 3; T3 separates upper mudstones of sheet 3 from siliceous mudstones and cherts of sheet 4 whose stratigraphic topping direction is overturned compared to the other sheets.

Fault zones are 10–50 metres in thickness and mostly accommodate strain in the weaker clay-rich lithologies (siliceous mudstones and siliceous claystones), typically localizing deformation along carbonaceous-material-rich layers. A pervasive foliation in the siliceous mudstones of T1 and 50–100 cm thick slip zones with scaly fabric in siliceous claystones and siliceous mudstone suggest predominant deformation by aseismic creep. The stiffer cherts are also involved in the fault zones. In T1, the hanging-wall derived brecciated cherts host a mm-thick pseudotachylyte fault vein recording earthquake slip [2]. In T3 a localized fault core in the hanging-wall cherts is rich in quartz clasts with pervasive 2-5 µm spaced deformation lamellae, recording high stress pulses.

Chlorite geothermometry applied on syn-kinematic chlorite and chlorite-quartz veins abundant in the fault rocks provide temperatures in the range 170–210 °C, in line with peak condition estimates for the area, confirming that the investigated structures were developed during accretion. Lower chlorite temperatures, down to 100°C, have also been measured in a scaly fabric fault zone, suggesting later reactivations of the fault at colder (shallower) conditions during exhumation.

These preliminary results highlight the importance of the heterogeneous stratigraphy of accretionary complexes in controlling faulting style: while weak mudstones accommodated most of slip by aseismic creep, the stiffer cherts hosted occasional high-stress pulses associated with seismic ruptures. Further questions to answer include how slip is partitioned and what factors promote seismic ruptures in the stiffer lithologies.

 

[1] Kimura, K., Hori, R. (1993) Journal of Structural Geology, 15(2), 145-161.

[2] Ujiie, K., et al. (2021) Earth and Planetary Science letters, 554, 11638

How to cite: Toffol, G., Robertson, R. V. M., Fagereng, Å., Ujiie, K., and Julve Lillo, J.: Accretionary complex heterogeneity controls the faulting style of upper plate thrusts, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17287, https://doi.org/10.5194/egusphere-egu26-17287, 2026.

EGU26-18134 | Posters on site | TS3.3

Tectonic transition in the northeastern Tibetan Plateau: from tectonic escape to mountain building 

Mian Liu, Shunying Hong, and Yuhang Li

The northeastern Tibetan Plateau is bounded by two major left-lateral strike-slip faults: the Altyn Tagh and Haiyuan faults. Eastward crustal motion along these faults, driven by the ongoing Indo-Asian continental collision, diminishes progressively toward their eastern terminations. Here, the crustal deformation is dominated by crustal shortening, thrust faulting, and uplift, which collectively contribute to the lateral growth of the plateau. Understanding this tectonic transition is essential for interpreting the plateau’s expansion and the seismic hazard along its northeastern boundary. We integrated InSAR, GNSS, and precise-leveling data to reveal the present-day crustal deformation in the northeastern Tibetan Plateau. Our analysis indicates that eastward motion along the Altyn Tagh fault is absorbed by thrusting and uplift within the Qilian Shan. Similarly, the Haiyuan fault transitions into crustal shortening and uplift in the Liupan Shan orogen. These transitions are largely controlled by the geometry of the strike-slip faults and the presence of the rigid Alashan and Ordos blocks to the east, which impede eastward motion of the Tibetan crust. Our results of present-day crustal deformation align with late-Cenozoic geological structures in northeastern Tibet and the stress patterns inferred from earthquakes along its northeastern margins, supporting a consistent model of ongoing plateau growth through transitioning from the escaping tectonics to mountain building.

How to cite: Liu, M., Hong, S., and Li, Y.: Tectonic transition in the northeastern Tibetan Plateau: from tectonic escape to mountain building, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18134, https://doi.org/10.5194/egusphere-egu26-18134, 2026.

EGU26-19671 | ECS | Orals | TS3.3

 Seismic–Aseismic Slip Partitioning on a Frictionally Heterogeneous Fault: An Experimental Approach 

Nico Bigaroni, Julian Mecklenburgh, and Ernest Rutter

Faults in the shallow brittle crust are rarely frictionally homogeneous. Structural and mineralogical heterogeneities such as phyllosilicate-rich shear zones mixed with competent lenses generate, respectively, velocity-strengthening (VS) and velocity-weakening (VW) domains that strongly influence earthquake nucleation and rupture dynamics. Geological observations and laboratory experiments show that VW patches typically nucleate unstable stick-slip, whereas VS regions promote stable creep and can transfer stress on neighbouring VW patches. Although this heterogeneous patch framework supports models of shallow seismicity, induced seismicity, and subduction zones, direct experimental investigations with rock samples and realistic patch geometries remain limited.

Here we present a new experimental framework for testing heterogeneous fault slip in cm-scale rock samples. Using the newly developed “BeeAx” servo-controlled biaxial apparatus, we sheared 15 × 17 cm Pennant Sandstone blocks at slow displacement rates (~1 µm/s) and 2, 5 and 8 MPa of normal stress. We compare three frictional sliding configurations: (1) homogeneous sandstone–sandstone (VW-dominated), (2) homogeneous graphite-coated sandstone (VS-dominated), and (3) heterogeneous samples with four circular uncoated sandstone patches embedded within a graphite background, comprising 50% of the sliding surface. High-resolution and calibrated acoustic emission (AE) monitoring (16 sensors) allows hypocentre location and source parameter retrieval, enabling direct comparison of microseismicity and frictional stability across configurations.

The homogeneous graphite experiment produced stable sliding with very low friction (µ≈0.15), while the homogeneous sandstone samples exhibited unstable stick-slip and higher friction (µ≈0.5). The heterogeneous samples displayed hybrid behaviour: a low overall friction (µ≈0.20) comparable to graphite, yet persistent dynamic stick-slip events. AE hypocentres concentrated on the sandstone patches perimeters, revealing that aseismic creep in the weak graphite transfers shear stress onto the stronger patches, which subsequently fail seismically. Compared to homogeneous sandstone, heterogeneous samples showed larger stress drops, stronger localization of microseismicity, and reduced Gutenberg-Richter b-values. Temporal b-value evolution differed between configurations: constant and low for graphite, cyclic for sandstone (decreasing during interseismic loading and increasing post-mainshock), and intermediate but systematically lower in the heterogeneous case, consistent with enhanced stress transfer and patch interaction.

These results demonstrate that discrete weak VS regions can modulate and even enhance the seismicity of stronger VW patches by acting as creeping load reservoirs. This provides laboratory support for models invoking patchy asperities on shallow faults and in induced seismicity settings, where strong and weak rock patches coexist within a fault. More broadly, the experimental platform enables controlled studies of rupture nucleation, asperity geometry, interaction, and seismicity evolution in frictionally heterogeneous fault systems.

How to cite: Bigaroni, N., Mecklenburgh, J., and Rutter, E.:  Seismic–Aseismic Slip Partitioning on a Frictionally Heterogeneous Fault: An Experimental Approach, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19671, https://doi.org/10.5194/egusphere-egu26-19671, 2026.

EGU26-1317 | ECS | Posters on site | ERE5.1

Cumulative Controls on Intermediate-Field Seismic Migration: Comparative Evidence from Three Geothermal Stimulation Campaigns 

Zhiwei Wang, Kristine Pankow, Antonio Rinaldi, James Verdon, and Ian Main

Injection-induced seismicity in Enhanced Geothermal Systems (EGS) can migrate hundreds of meters from the well and often persists after shut-in, raising operational and hazard concerns. Here we present a cross-site comparative analysis of three stimulation campaigns—Soultz-sous-Forêts (France, 1993), Basel (Switzerland, 2006), and Utah FORGE Stage 3 (USA, 2022)—to identify the dominant controls on intermediate-field seismic migration.

Using a unified dynamic time-windowing framework, we track seismic front evolution via three complementary distance metrics and evaluate their relationships with injection rate, wellhead pressure, cumulative injected volume, hydraulic energy, seismicity rate, and modeled pore pressure at the migration front. Across all sites, cumulative variables—particularly injected volume, hydraulic energy, and injection duration—show the strongest and most consistent correlations with seismic front expansion, whereas instantaneous parameters exhibit weaker or site-specific influence.

Post-injection behaviors distinguish three migration regimes: (i) a pressure-limited regime at Soultz, where the front halts immediately after shut-in; (ii) a diffusion-dominated regime at Basel, with continued post-shut-in propagation; and (iii) a stress-sensitive, limited-diffusion regime at Utah FORGE, characterized by rapid early migration followed by stagnation. Building on these contrasts, we introduce a six-indicator radar classification that quantitatively distinguishes the three regimes.

Our results show that cumulative hydraulic forcing provides transferable, physically interpretable predictors of intermediate-field migration and that distinct post-shut-in signatures reflect underlying connectivity and stress conditions. This comparative framework supports improved seismic hazard assessment and operational planning for geothermal reservoir stimulation.

How to cite: Wang, Z., Pankow, K., Rinaldi, A., Verdon, J., and Main, I.: Cumulative Controls on Intermediate-Field Seismic Migration: Comparative Evidence from Three Geothermal Stimulation Campaigns, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1317, https://doi.org/10.5194/egusphere-egu26-1317, 2026.

EGU26-1912 | ECS | Orals | ERE5.1

Assessing induced seismicity risk for the Lower Yarlung Tsangpo hydropower complex 

Haonan Wang, Shemin Ge, and Xiaodong Ma

A large hydropower complex is planned on the Lower Yarlung Tsangpo (YT) with an expected output roughly three times that of the Three Gorges Project. The planned hydropower complex lies in the eastern Himalayan syntaxis, which is characteristic of intricate fault systems, high tectonic strain rates, and strong topographic variations. Reservoir impoundment in such a geologic setting may lead to unintended consequences such as induced seismicity and landslides. A pre-impoundment risk assessment is imperative for the region and the project. With regional faults and stress information, we perform an analysis to identify the fault segments that may be affected by reservoir impoundment and lead to seismicity.
The existing observations from hydraulic fracturing tests indicate that the rotation of SHmax orientation shows similarities with the changes in the YT course. To obtain abundant and diverse stress information, we compiled 145 focal mechanisms for the study area covering the period of 2000 - 2023. Moment magnitudes concentrate around 1.5 - 4, and hypocenter depths are in the upper crust (≤ 15 km). Given the complexity of the fault system and the pronounced heterogeneity in the number and distribution of focal mechanisms, we partitioned the study area into four subregions and performed focal mechanism stress inversions separately for each subregion. The inversion results reveal a strike-slip regime in three subregions and a thrust faulting regime in one subregion. The stress ratios for all subregions lie in the range 0.6 - 0.8. The inverted SHmax orientations differ markedly between subregions, with a maximum discrepancy of ~58.5°.
To quantify fault destabilization risk, we employ a parameter termed ‘fault instability’ (FI). The FI range is from 0 to 1, ‘0’ for the most stable fault, while ‘1’ for the most unstable fault. It is quantified by fault frictional coefficient μf, fault strike and dip, stress field, and pore pressure. To consider the uncertainty in these input parameters, the Monte Carlo sampling is used to constrain the FI. Different fault segments exhibit markedly different FI values. Seismicity over the 23-year period predominantly occur on faults with high FI values, corroborating the qualification of the FI. FI distribution can inform dam siting and tunnel routing. We plan to build a 3D hydro-mechanical model that couples observed and inverted geological data, simulate pore pressure diffusion and water loading effects on Coulomb stress, and assess the resulting changes in FI and induced seismicity risk.

How to cite: Wang, H., Ge, S., and Ma, X.: Assessing induced seismicity risk for the Lower Yarlung Tsangpo hydropower complex, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1912, https://doi.org/10.5194/egusphere-egu26-1912, 2026.

EGU26-2227 | ECS | Posters on site | ERE5.1

 The Dual Role of Ductile Barriers: From Stress-Concentrating Seals to Coseismic Valves in Induced Seismicity 

Junhao Tao, Xinxing Chen, Diai Liu, Haichao Chen, Yang Zhao, Fenglin Niu, and Laibin Zhang

Hydraulic fracturing often induces complex seismic sequences that migrate across stratigraphically distinct formations. However, the mechanisms governing delayed triggering and vertical interaction through lithological boundaries remain poorly understood. In this study, we report a novel "coseismic valve" mechanism observed in the Weiyuan shale gas field, southern Sichuan Basin, where the multi-stage evolution of seismicity was strictly governed by pre-existing 3D mechanical stratigraphy.

Using a dense local monitoring array, we constructed a high-resolution catalog by the deep-learning-based LOC-FLOW workflow. This catalog revealed a vertically partitioned fault system, where the deep and shallow seismicity clusters are distinctly separated by a ~400 m thick low-velocity ductile barrier.This barrier mechanically isolated a deep, critically stressed segment (characterized by a low b-value) from a shallower, compliant damage zone. Our analysis reveals a paradox in the role of ductile layers: initially, the barrier acted as a "pressure seal," preventing fluid leak-off and facilitating high differential stress accumulation in the underlying reservoir. This confinement culminated in the nucleation of an Mw 3.6 mainshock with an anomalously high stress drop.

Crucially, finite fault inversion and isochrone back-projection demonstrate that the mainshock rupture propagated upward, dynamically breaching the ductile barrier. This mechanical breach effectively functioned as a valve, establishing a vertical conduit for hydraulic connectivity. Following a distinct 6-day delay, a diffusive seismic swarm erupted in the previously quiescent shallow segment, driven by the upward surge of overpressured fluids through the newly created fracture network.

Our findings challenge the conventional view of ductile layers merely as passive aseismic buffers. We demonstrate that they can play a dual role: serving as stress-concentrating seals that prime the system for nucleation, and as structural valves that, once ruptured, enable cascading seismic hazards. This dynamic interaction highlights the necessity of integrating 3D structural frameworks into seismic risk assessment for geo-energy projects.

How to cite: Tao, J., Chen, X., Liu, D., Chen, H., Zhao, Y., Niu, F., and Zhang, L.:  The Dual Role of Ductile Barriers: From Stress-Concentrating Seals to Coseismic Valves in Induced Seismicity, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2227, https://doi.org/10.5194/egusphere-egu26-2227, 2026.

Hydraulic fracturing operations in the Southern Sichuan Basin have generated significant induced seismicity, raising important questions about the underlying rupture processes. We analyze stress drops of 3,369 induced earthquakes (ML > 0.5) using a non-parametric generalized inversion technique with rigorous reference-station corrections. Our analysis reveals two key characteristics of these induced events: first, they exhibit systematically low stress drops (median 0.07 MPa) that show positive scaling with seismic moment, challenging classical self-similarity assumptions; second, we observe pronounced spatial variations in stress release that correlate with depth and fault structure. Notably, fluid diffusion drives rapid activation of fault asperities, resulting in repeated high-stress-drop ruptures (0.3-6.0 MPa) within short timescales of days. This accelerated rupture cycle differs fundamentally from tectonic earthquake recurrence patterns. Our findings demonstrate that induced earthquake rupture dynamics are controlled by the interplay of heterogeneous fault strength and rapid fluid pressurization, providing critical insights for developing targeted hazard assessment strategies in energy-producing regions.

How to cite: Chen, X., Tao, J., Liu, D., and Chen, H.: Stress Drop Variability and Rapid Fault Activation in Hydraulic-Fracturing-Induced Earthquakes: Insights from the Southern Sichuan Basin, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2228, https://doi.org/10.5194/egusphere-egu26-2228, 2026.

During the siting of hydraulic-fracturing (HF) wells within industrial activity areas, identifying potential seismogenic faults and effectively avoiding them is critical for mitigating induced seismicity risk. Meanwhile, characterizing the fine-scale structures of seismogenic faults provides the essential foundation for analyses of the mechanisms and rupture processes of induced earthquakes. However, multiple case studies have demonstrated that, even where seismic reflection data are available, it remains difficult to identify small-displacement seismogenic faults, particularly those dominated by strike-slip faults. Consistently, the four representative M5+ induced earthquakes in the Changning and Weiyuan shale gas blocks of the Sichuan Basin also exhibit difficulties in identifying the seismogenic faults from seismic reflection data. Moreover, the scales of faults that can be identified through seismic reflection data and related interpretation methods, and their corresponding seismogenic potential, remain to be systematically defined and quantitatively constrained. This study integrates spatiotemporal data from HF operations, seismicity data, and high-resolution 3D seismic reflection data, together with surface deformation measurements, to address the above questions.

The results show that potential seismogenic faults with moment magnitude (Mw) greater than approximately 3.3 that displace strong reflection horizons can be effectively identified using high-resolution 3D seismic reflection data. In addition, the associated structures of small-displacement strike-slip faults facilitate their recognition in seismic reflection profiles. A common feature of the seismogenic fault systems of the four representative earthquakes is that small-displacement subsidiary faults (including strike-slip faults) intersect the fracturing wells within the reservoir interval, forming downward migration pathways for fracturing fluids and thereby activating the underlying thrust or strike-slip seismogenic faults. More importantly, such small-displacement faults are widely developed within the fractured intervals of the Sichuan Basin shale gas fields, yet their identification remains challenging. As a result, numerous horizontal wells intersect these faults, constituting a key reason for the frequent occurrence of induced seismicity in these areas. The most effective approach to recognizing these faults is to trace multiple strong reflection horizons to construct structural maps. By applying multi-azimuth illumination and vertical stretching, fault traces can be visualized more clearly, in combination with various types of seismic reflection attribute volumes.

Beyond the Sichuan Basin, injection-induced earthquakes in most shale gas fields worldwide are also closely associated with small-displacement faults, particularly strike-slip faults. The failure to avoid such faults during the siting of HF wells is also likely a major reason for the frequent occurrence of induced seismicity in these areas. The small-displacement fault identification techniques presented in this study facilitate a more precise delineation of seismogenic fault system structure. More importantly, during well site selection, from the perspective of fault identification and avoidance based on 3D seismic reflection data, this study provides theoretical support and practical strategies for preventing induced earthquakes with a magnitude (Mw) greater than approximately 3.3. These findings also offer significant implications for the prevention of induced seismicity caused by fluid/gas injection in a broader range of applications.

How to cite: Ye, Y. and Lu, R.: Identification and Impacts of Small-Displacement Faults in Industry-induced earthquake: Insights from the Southern Sichuan Shale Gas Field, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2497, https://doi.org/10.5194/egusphere-egu26-2497, 2026.

Identifying and distinguishing induced seismicity from background regional tectonic activity remains a major challenge within tectonically active settings, due to the overlap between natural seismicity and seismicity potentially triggered by human activities. Induced seismicity refers to earthquakes generated or modulated by anthropogenic processes such as reservoir impoundment, fluid injection or extraction, and mining. While mining-induced seismicity has been shown to increase seismicity rates and magnitudes in tectonically stable regions, fundamental uncertainties remain regarding the spatial extent of mining influence and its detectability in areas with high background tectonic activity. The case of study is in the Central Andes (18-36°S), in the Chilean Andean Margin. Here, long-lived subduction has shaped well-defined metallogenic belts hosting major metallic ore deposits, within which Chile has developed a long history of open-pit and underground mining across diverse geological and operational settings. We use regional crustal seismicity from a recently published regional seismic catalog, together with a database of large-scale open-pit and underground mining operations in Chile, to systematically evaluate spatial and statistical relationships between seismicity patterns and mining activity. Specifically, we apply a three-phase framework to identify seismic events with a higher likelihood of mining-induced origin. We first define a 15 km depth threshold to separate shallow seismicity potentially influenced by mining from deeper regional tectonic events, and distinguish near-field from far-field seismicity based on proximity to mining operations. We then apply a nearest-neighbor clustering method to identify stochastically independent events, which are more likely to be induced. Finally, distance to mines and clustering information are combined into a linear weighted metric that quantifies the likelihood of induced seismicity. The results reveal a marked daily temporal anomaly in shallow seismic behavior (depth < 15 km), where an increase in activity is observed in the near field of mines between 16:00 and 22:00, aligning with the mines’ primary operational windows and blasting schedules. Within this time window, the probability of events belonging to a tectonic cluster decreases, thereby increasing the likelihood that they are induced seismicity rather than aftershock sequences. The primary finding highlights a daily six-hour window that concentrates 70% of the total seismic activity in the near field of mines. This represents a concentration 2.8 times higher than normal compared to regional seismicity, which lacks a preferred time frame. These observations indicate that mining activities can impose a measurable temporal signature on seismicity, even within a tectonically active subduction margin, contributing to the broader understanding of how anthropogenic processes interact with natural seismic systems.

How to cite: Ravest, B. and Roquer, T.: Spatial and Temporal Metrics for the Identification of Mining-Induced Seismicity: The Case of the Chilean Andean Margin, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4084, https://doi.org/10.5194/egusphere-egu26-4084, 2026.

EGU26-6012 | Orals | ERE5.1

Shear slip and opening of existing faults during fluid injection: insights from tilt measurements 

Saeed Salimzadeh, Aurora Lambiase, Valentin Gischig, Dane Kasperczyk, Men-Andrin Meier, Marian Hertrich, and Antonio Rinaldi

Fluid injection in the subsurface for the purpose of CO2 sequestration, geothermal heat extraction or energy storage has frequently caused faults activation and seismicity, raised the communities’ concerns and ultimately resulted in project shutdown. In order to understand earthquakes, a set of unique experiments are being conducted in Bedretto Underground Laboratory for Geosciences and Geoenergy located at 1,000 m depth under the Swiss Alps. In these suites of experiments, small-scale non-damaging earthquakes are induced via water injection into a well-known and well-characterised fault.

A set of three borehole tiltmeters were deployed in the vicinity of the injection borehole and its data were used for analysing the fault’s behaviour during and after injection. A 3D finite element model (CSMP-HF) was utilised to predict the tilt vectors at specified stations from a set of prescribed input data (geometry, loading, stiffness, etc.), and a residual (cost) function was defined based on Bayesian framework to evaluate the closeness of the model predictions to the field measurements. Finally, a Differential Evolution optimisation technique was used to locate the global minima of the residual (cost) function, corresponding to the best set of input data. The inversion model results confirmed that both shear slip and opening (dilation) deformations occurred not only on the target fault, but also on another transverse fault. The inversion model was capable of accurately finding the location of “unknown” secondary fault which was consistent with log data gathered from another observation wellbore. The shear slippage consisted of both dip-slip (vertical) and strike-slip (horizontal) deformation, consistent with measured in-situ stresses.

How to cite: Salimzadeh, S., Lambiase, A., Gischig, V., Kasperczyk, D., Meier, M.-A., Hertrich, M., and Rinaldi, A.: Shear slip and opening of existing faults during fluid injection: insights from tilt measurements, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6012, https://doi.org/10.5194/egusphere-egu26-6012, 2026.

EGU26-7196 | ECS | Orals | ERE5.1

Multi-scale Characterization of Seismic Noise and Signals in an Underground Coal Mine 

Patchamatla V M V Prasada Raju and Paresh Nath Singha Roy

Seismic monitoring in underground coal mining environments is influenced by various anthropogenic and natural noise sources. The background noise, predominantly of mechanical origin, shows strong spatial and temporal variability. Some highly impulsive sources share common characteristics with genuine seismic events. Routine blasting activities within the mine and from surrounding regions also contribute significantly to the recorded data. Mining-triggered sources such as microseismicity, subsidence, roof falls, and occasional sensing of tectonic earthquakes originating from distant locations further contribute to the recorded data. The combined influence of these sources strongly affects the performance of conventional processing workflows, frequently resulting in false detections and event misclassifications.

In this study, continuous seismic data recorded in an underground coal mine using eight short-period seismometers over a six-month duration are analysed to characterise signal and noise properties across temporal, spectral, and spatial domains. Spectral persistence, correlation metrics, and multichannel signal-processing techniques are used to identify dominant noise sources and assess their influence on the recorded waveforms. Persistent mechanical activity is shown to dominate the spectrum, with numerous harmonics and broadband noise, motivating the use of multiscale decomposition methods.

We evaluate the performance of Empirical Mode Decomposition (EMD) and Variational Mode Decomposition (VMD) for multiscale analysis. Our results show that EMD can introduce spurious low-frequency modes that are absent from the original signals and can therefore be misinterpreted. In contrast, VMD’s constrained-bandwidth formulation yields more physically meaningful scale separation. The multivariate extension of VMD (MVMD) has been used for better mode alignment and correlation across channels.

Overall, these results demonstrate the advantages of constrained, multivariate multiscale methods for the characterization of signal and noise with implications for improving seismic monitoring and event classification in complex environments.

 

How to cite: Prasada Raju, P. V. M. V. and Roy, P. N. S.: Multi-scale Characterization of Seismic Noise and Signals in an Underground Coal Mine, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7196, https://doi.org/10.5194/egusphere-egu26-7196, 2026.

EGU26-8098 | ECS | Posters on site | ERE5.1

Characterization of microseismicity at the Húsmúli reinjection area, Hengill Geothermal Field, Southwest Iceland​ 

Sargun Kaur, Tania Toledo, Toni Kraft, and Verena Simon

Induced seismicity remains a major challenge for geothermal projects, with implications for public acceptance and operational risk management. Understanding how fluid injection interacts with fault structures to generate seismicity is therefore essential. The Húsmúli reinjection area in the Hengill geothermal field (SW Iceland) provides an ideal setting to investigate these processes due to its sustained induced seismicity and long operational history. Here, we present an improved seismicity catalog (2018–2021; COSEISMIQ project) and a waveform-based detection workflow that substantially increases catalog completeness and enhances spatiotemporal resolution.

We first improve the initial automatic catalog by re-picking events with unrealistic Vp/Vs ratios (Wadati analysis), high RMS location misfits, or unrealistic depths (e.g., airquakes). Phase picks are then refined using a cross-correlation (CC)-based repicking approach: events are clustered into waveform-similar families, traces are aligned and stacked to increase signal-to-noise, and consistent arrival times are obtained from a single-family reference pick. Missing picks are recovered by inspecting waveforms around the expected arrival time window and estimating phase onsets, accepting only traces with  CC ≥ 0.65 with respect to other family members.

3D spatial clustering of the refined catalog reveals NE–SW oriented seismic lineaments consistent with mapped faults and inferred fluid migration pathways. In contrast, nearby E-W structures show little to no seismicity, suggesting permeability barriers and reservoir compartmentalization. Repeating earthquakes occur along narrow fault segments, indicating repeated rupture of localized slip patches. To further enhance detection, we use QuakeMatch, a single-station template matching workflow using high-SNR events as templates at the station with the best waveform quality and data completeness. This expands the catalog from 3,647 to 12,899 events, lowering the magnitude of completeness and revealing numerous low-magnitude earthquakes previously missed by the automatic STA/LTA processing due to low signal-to-noise or waveform overlap. The resulting catalog shows swarm-like activity typical of fluid-driven seismicity and episodic bursts. A prominent sequence on 15 November 2020 (MLX  = 4.08) is preceded by foreshocks and followed by multiple MLX ≥ 3.0 aftershocks. Gutenberg–Richter analysis indicates a decrease in b-values prior to the mainshock, consistent with stress build-up and suggesting potential precursory behaviour relevant for operational monitoring.

How to cite: Kaur, S., Toledo, T., Kraft, T., and Simon, V.: Characterization of microseismicity at the Húsmúli reinjection area, Hengill Geothermal Field, Southwest Iceland​, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8098, https://doi.org/10.5194/egusphere-egu26-8098, 2026.

EGU26-8208 | ECS | Orals | ERE5.1

Nucleation and rupture of induced earthquakes in Groningen confined to the gas reservoir 

Meng Li, Andre R Niemeijer, Femke C Vossepoel, and Ylona van Dinther

To assess seismic hazard in the Groningen gas field, it is crucial to understand earthquake source processes, including the locations of nucleation and possible arrest. These fundamental characteristics, however, remain poorly constrained by seismological observations due to limited resolution. Interpretations of seismological observations are often inconsistent because the focal depth inversion uncertainty (~300 m) is comparable to reservoir thickness (50-300 m). Two fault segments, the velocity-weakening anhydrite layer within the caprock sequence and the velocity-strengthening sandstone reservoir experiencing substantial healing, are suggested to be seismogenic [1]. However, their respective roles in nucleation and rupture remain unclear. Additionally, whether ruptures can propagate into the over- and underburden layers is also debated, yet this is a key constraint for the maximum possible earthquake magnitude (Mmax).

 

Here, we use physics-based earthquake sequence simulations to investigate how stratigraphic layering, lithology-dependent elastic and frictional properties, and long-term fault healing govern rupture behavior. We find that earthquake nucleation consistently occurs within the sandstone reservoir, even when velocity-weakening friction is assigned to the overlying anhydrite caprock. Rupture propagation is predominantly confined to the reservoir thickness, with only limited penetration into adjacent formations. The anhydrite can only be activated, in rare cases, through rupture propagation. Introducing mechanical heterogeneity exerts a dominant control on rupture behavior by substantially suppressing slip rates and limiting rupture extent, whereas frictional heterogeneity has a comparatively minor effect in the opposite sense. Fully runaway rupture into the underburden is exceedingly rare. It only occurs in one out of 2,000 simulations and requires an extreme and unlikely combination of geometric, mechanical, and frictional conditions. Statistical mapping of simulation outcomes onto the Groningen fault network indicates that most fault segments have 5% or less likelihood of rupture propagating over a distance larger than the reservoir thickness. The likelihood of fully runaway rupture is 0.3%–1% only in a few peripheral regions beyond the locus of recorded earthquake occurrence and below 0.3% elsewhere. Together, these results demonstrate that lithological heterogeneity imposes strong physical constraints on rupture extent, providing robust, physics-based limits on Mmax and improving seismic hazard assessment for Groningen and other energy-producing regions.

 

[1] Li, M., Niemeijer, A., Van Dinther, Y. (2025, Nat. Comm.) https://doi.org/10.1038/s41467-025-63482-3.

How to cite: Li, M., Niemeijer, A. R., Vossepoel, F. C., and van Dinther, Y.: Nucleation and rupture of induced earthquakes in Groningen confined to the gas reservoir, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8208, https://doi.org/10.5194/egusphere-egu26-8208, 2026.

EGU26-8567 | Orals | ERE5.1

Elevated in-situ Vp/Vs preceding M > 3 hydraulic-fracturing induced earthquakes  

Jian Xu, Yajing Liu, Junlun Li, Marco Roth, Rebecca Harrington, and Yicheng He

Hydraulic-fracturing (HF) induced seismicity has attracted growing global attention, with the recorded maximum magnitudes reaching up to M6.0 in the southern Sichuan basin, China. How to mitigate the induced seismic hazard is key for safe energy development. Three mechanisms are proposed to explain earthquake triggering during HF: fluid diffusion, poroelastic stress perturbations, and aseismic slip, which can act individually or in combination. Although fluid diffusion is widely regarded as the primary driver, tracking pore-pressure evolution in near real time and quantifying its role in the nucleation of moderate-to-strong earthquakes remains challenging. Here we apply a non-tomographic Vp/Vs method (Lin and Shearer, 2007) to the southern Sichuan Basin, China and analyze the spatiotemporal variations of near-source Vp/Vs during three moderate M3-M4 HF induced earthquake sequences. Benefiting from abundant clustered induced seismicity and dense seismic arrays, we resolve Vp/Vs changes at a high resolution of ~2 days and ~150 m. We observe a consistent increase in Vp/Vs from ~1.73 to ~1.80 prior to the moderate-sized earthquakes, suggesting progressive pore-pressure buildup that culminates in seismic slip. In addition, the elevated pore pressure precedes eventual seismic slip by ~5–10 days, highlighting a preparatory phase for earthquake nucleation, which could be a valuable time window for making injection parameter adjustments to mitigate seismic hazard. The ability to resolve observable changes that precede moderate seismic events on such time scales suggests that the in-situ Vp/Vs approach offers a promising near-real-time monitoring strategy for seismic hazard assessment in a HF setting.

How to cite: Xu, J., Liu, Y., Li, J., Roth, M., Harrington, R., and He, Y.: Elevated in-situ Vp/Vs preceding M > 3 hydraulic-fracturing induced earthquakes , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8567, https://doi.org/10.5194/egusphere-egu26-8567, 2026.

EGU26-8716 | ECS | Posters on site | ERE5.1

HydroMech3D: physics-based earthquake-cycle modeling of fluid-driven fault slip with realistic fault geometry 

Zhenhuan Wang, Luca Dal Zilio, Federico Ciardo, and Antonio Rinaldi

Fluid injection associated with geoenergy applications such as geothermal energy, CO2 sequestration, and hydraulic fracturing can alter fault stability through a combination of coupled hydro-mechanical processes. Laboratory experiments and underground observatories have provided valuable constraints on fault friction and near-fault pressure evolution, yet translating these observations to field-scale behavior requires physics-based numerical models that can resolve fault slip under realistic geometrical and mechanical conditions.

A major limitation of existing modeling approaches is the high computational cost of fully coupled three-dimensional simulations. As a result, many studies rely on one-dimensional fault representations or simplified elastic and hydraulic coupling. While such models have provided important insights into key physical mechanisms, they are not well suited to support the design, interpretation, and long-term forecasting of modern injection experiments equipped with dense monitoring systems. These experimental settings increasingly demand three-dimensional models capable of capturing realistic fault geometry, spatially variable frictional and hydraulic properties, and stress interactions beyond reduced-dimensional assumptions.

Here we present HydroMech3D, a physics-based numerical framework designed to efficiently simulate fluid-driven fault slip over earthquake-cycle timescales in three dimensions. The model employs a quasi-dynamic Boundary Element Method, discretizing only the fault surface embedded in elastic medium, thereby avoiding volumetric meshing. Fault slip is governed by rate-and-state friction and coupled to pore-pressure diffusion along the fault. Computational efficiency is achieved through a C++ implementation accelerated by hierarchical matrix from the Bigwham Library, enabling large-scale simulations with realistic fault geometry.

This framework allows systematic investigation of fault-scale heterogeneity, including asperities with contrasting frictional and hydraulic properties, and provides a platform to explore how three-dimensional fault structure influences aseismic slip, stress transfer, and earthquake nucleation during fluid injection. Benchmarking against established earthquake-cycle test cases validates the mechanical solver and establishes a baseline for ongoing fully coupled simulations. HydroMech3D offers a computationally efficient open-source tool to support experiment design, interpretation of near-fault observations, and assessment of induced seismicity in geoenergy applications.

How to cite: Wang, Z., Dal Zilio, L., Ciardo, F., and Rinaldi, A.: HydroMech3D: physics-based earthquake-cycle modeling of fluid-driven fault slip with realistic fault geometry, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8716, https://doi.org/10.5194/egusphere-egu26-8716, 2026.

EGU26-9185 | Posters on site | ERE5.1

Variability of the Seismic Response of the Rittershoffen Geothermal Reservoir to the Series of GRT-1 Stimulations 

Emmanuel Gaucher, Olivier Lengliné, and Jean Schmittbuhl

Between April and June 2013, the GRT-1 well at the Rittershoffen geothermal site in the Upper Rhine Valley (France) underwent three distinct stimulation phases: first a thermal stimulation, then a chemical stimulation, and finally a hydraulic stimulation. These fluid injections significantly enhanced the injectivity index of the well, rendering it suitable for economic exploitation. Throughout these operations, a local surface seismic network continuously monitored the site, recording thousands of unfelt seismic events.

This study builds upon and refines the findings of Lengliné et al. (2017), who focused solely on the hydraulic stimulation of GRT-1, and Maurer et al. (2020), whose interpretations were constrained by uncertain absolute locations of seismic events, particularly in terms of depth. By employing an improved template matching technique and a relative location method, we established a comprehensive seismic event catalog comprising over 3,000 events.

This reliable catalog enables precise tracking of the reservoir’s seismogenic response to the successive yet distinct stimulation types, with high spatial and temporal resolution. Consequently, it allows for an investigation into the potential seismic interplay between these stimulations. Our analysis examines the evolution of key characteristics, including event distribution and clustering, b-value, and seismic injection efficiency across the stimulation phases. The observed differences prompt critical questions regarding the reliability of using responses from prior stimulations to forecast seismogenic behavior during subsequent operations, even for the same site.

How to cite: Gaucher, E., Lengliné, O., and Schmittbuhl, J.: Variability of the Seismic Response of the Rittershoffen Geothermal Reservoir to the Series of GRT-1 Stimulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9185, https://doi.org/10.5194/egusphere-egu26-9185, 2026.

EGU26-9772 | ECS | Posters on site | ERE5.1

Injection-induced seismicity fronts and stress distribution on rough faults 

Hsiao-Fan Lin, Thibault Candela, and Jean-Paul Ampuero

The increasing occurrence of injection-induced earthquakes has raised public concern and highlighted the importance of understanding subsurface processes to assess induced seismic hazards and risks. A feature of natural faults that has not received sufficient attention in induced seismicity modeling is their geometric roughness. We develop a simple physics-based model to investigate how fault roughness can control induced seismicity during fluid injection.

The first approach to modeling along-fault stresses prior to injection is to project the background stress tensor onto the rough fault. In this case, our models and theoretical analysis show that the apparent diffusivity of seismicity fronts can deviate significantly from the hydraulic diffusivity. Faults with realistic roughness generally display slow seismicity migration, producing apparent diffusivities far below the hydraulic values. Thus, seismicity fronts often lag behind the pressure front, especially at low background stresses and small roughness amplitudes. Only in the rare case of very rough faults stressed very close to failure, apparent diffusivity can exceed the hydraulic diffusivity, leading to seismicity fronts that outpace pressure fronts. 

The second approach to modeling along-fault stresses prior to injection is to simulate stress evolution after multiple tectonic rupture cycles. This ongoing work explores the resulting stress heterogeneity after multiple tectonic rupture cycles and examines whether seismicity migration follows the same trend as in the first approach, i.e., whether seismicity migration is generally slower than the pressure front on rough faults.

Apart from seismicity migration, the magnitude-frequency statistics are also analyzed. Along this single rough fault the frequency-magnitude distribution is bimodal. These results demonstrate how fault roughness and stress conditions control the induced seismicity through their influence on the criticality of the fault and stress transfer, and link long-term fault loading processes with short-term seismicity migration patterns in fluid injection scenarios.

How to cite: Lin, H.-F., Candela, T., and Ampuero, J.-P.: Injection-induced seismicity fronts and stress distribution on rough faults, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9772, https://doi.org/10.5194/egusphere-egu26-9772, 2026.

EGU26-11254 | ECS | Orals | ERE5.1

Investigating fracture and stress controls on induced seismicity in geothermal reservoirs with a coupled THM model 

Gaëlle Toussaint, Stephen A. Miller, and Benoît Valley

Enhanced Geothermal Systems (EGS) aim to provide sustainable energy by increasing the permeability of deep, low-productivity reservoirs through hydraulic stimulation. While micro-seismicity is an expected outcome of stimulation, larger induced earthquakes such as those recorded in Basel (2006) and Pohang (2017) remain a major challenge for the safe deployment of deep geothermal projects. This highlights the need for physics-based models capable of resolving the coupled processes and fault behavior that control induced seismicity, and of assessing how reservoir properties and stimulation strategies influence seismicity rates and maximum magnitudes.

We present a numerical framework designed to investigate how coupled thermo-hydro-mechanical (THM) processes govern fault reactivation and induced seismicity in EGS. The model explicitly couples fluid flow, heat transfer, and stress evolution, and incorporates stress-dependent deformation, fault reactivation, and a built-in earthquake detection algorithm based on deviatoric strain rate. This approach enables consistent identification of induced events within simulations and quantification of their magnitudes, providing a process-based framework to explore the spatio-temporal evolution of seismicity. To resolve fault complexity and process coupling at high spatial and temporal resolution, the model is implemented using high-performance computing tools, enabling efficient exploration of a wide range of scenarios.

Preliminary simulations of the 2006 Basel project reproduce key seismic characteristics, including b-values and maximum magnitudes consistent with observations. Early tests on different fracture networks indicate that fracture size strongly influences the resulting seismicity. Ongoing work systematically investigates the roles of fracture size, fracture criticality, and stress ratio in controlling induced seismic behavior. Overall, this modelling framework provides a flexible tool to explore the physical mechanisms driving induced seismicity in EGS and to support the development of safer stimulation strategies.

How to cite: Toussaint, G., Miller, S. A., and Valley, B.: Investigating fracture and stress controls on induced seismicity in geothermal reservoirs with a coupled THM model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11254, https://doi.org/10.5194/egusphere-egu26-11254, 2026.

EGU26-11445 | Orals | ERE5.1

Sedimentary heterogeneity and rock mechanical controls on reservoir compaction in the Groningen gas field 

Johannes Miocic, Sebastian Mulder, and Dmitry Bublik

Induced seismicity associated with gas production in the Groningen gas field, north-eastern Netherlands, underscores the need for improved forecasting of reservoir compaction and stress redistribution during long-term subsurface exploitation. While current geomechanical models typically assume laterally homogeneous reservoir properties, growing evidence suggests that sedimentary heterogeneity exerts a first-order control on sandstone compactional behaviour. This contribution integrates field-scale petrographic analysis with laboratory geomechanical experiments to quantify how inherited geological heterogeneity governs the mechanical response of the Permian Rotliegend reservoir.

A quantitative petrographic dataset of more than 300 samples from fifteen wells demonstrates that porosity loss across the field is overwhelmingly dominated by mechanical compaction associated with rapid Late Permian burial beneath the Zechstein evaporites, accounting for 55–95% of total porosity reduction. However, compaction efficiency varies systematically with depositional texture and early cementation rather than burial depth alone. Grain size, sorting, lamination, and early dolomite and anhydrite cementation controlled initial packing density and grain-contact geometry, leading to strong spatial heterogeneity in preserved intergranular volume and inferred mechanical properties.

To directly test the mechanical implications of this heterogeneity, we conducted triaxial deformation experiments on Rotliegend sandstones with comparable porosity (~12%) but contrasting cementation styles and clay contents. Experiments performed under reservoir-relevant stress and temperature conditions show that approximately 30% of total strain is inelastic, with time-dependent deformation occurring during stress relaxation phases. Samples containing higher clay contents accumulated the largest inelastic strain, while strongly dolomite- and quartz–anhydrite-cemented sandstones exhibited higher stiffness but still significant non-elastic deformation. Microstructural analyses using SEM reveal grain-scale damage patterns consistent with cement- and clay-controlled deformation mechanisms.

Together, these results demonstrate that reservoir compaction in Groningen is strongly conditioned by inherited sedimentary and diagenetic heterogeneity that is not captured in conventional homogeneous models. Incorporating these controls into geomechanical frameworks is essential for more realistic prediction of reservoir deformation and associated induced seismic hazard during subsurface resource exploitation.

How to cite: Miocic, J., Mulder, S., and Bublik, D.: Sedimentary heterogeneity and rock mechanical controls on reservoir compaction in the Groningen gas field, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11445, https://doi.org/10.5194/egusphere-egu26-11445, 2026.

EGU26-12093 | ECS | Orals | ERE5.1

Time-Lapse HVSR Analysis for Shallow Subsurface Monitoring at the CaMI.FRS CO2 Sequestration Site  

Tianyang Li, Tao Yu, Nian Yu, Yichun Yang, and Yu Jeffrey Gu

Seismic monitoring is a critical component of Carbon Capture and Storage (CCS) projects, ensuring the containment security of injected fluids and assessing the risks associated with induced seismicity. While fluid injection is known to alter effective stress and pore pressure—potentially inducing velocity changes or fault reactivation—distinguishing these deep subsurface signals from near-surface environmental variations remains a significant challenge. This study utilizes the passive source Horizontal-to-Vertical Spectral Ratio (HVSR) method to investigate the spatiotemporal variations of site response at the CO2 Containment and Monitoring Institute Field Research Station (CaMI.FRS) in Alberta, Canada, providing a robust baseline for long-term integrity monitoring. We analyzed continuous ambient noise data collected between September 2019 and October 2020 from a dense array of short-period seismic stations deployed around the injection well. The injection targets the Basal Belly River Formation at a depth of 300 m. Data processing involved dividing daily records into 150-second windows with 50% overlap, followed by bandpass filtering (0.2–20 Hz) and Konno-Ohmachi smoothing to calculate daily stability-weighted HVSR curves. The results reveal a consistent fundamental resonance frequency (f0) centered at approximately 2 Hz across the study area, corresponding to a soft sediment thickness of 100–150 m overlying the bedrock. While f0 remained relatively stable throughout the monitoring period, the H/V peak amplitude (amplification factor) exhibited significant seasonal time-varying characteristics. Specifically, a strong positive correlation was observed between the amplification factor and environmental variables, including atmospheric temperature, precipitation, and groundwater levels. The amplification factor reached its annual maximum (~2.5–2.6) during the warm, wet summer months (June–August) and dropped to its minimum (~1.5–1.8) during the frozen winter months. These findings suggest that variations in near-surface saturation and soil properties, driven by seasonal climate cycles, significantly modulate seismic site response. Consequently, for effective HVSR-based monitoring of deep CO2 plumes or leakage pathways, it is imperative to decouple these shallow environmental effects from the signals of deep geological alterations. This study demonstrates the efficacy of time-lapse HVSR as a low-cost, non-invasive tool for characterizing site response dynamics and highlights the necessity of multi-physics environmental calibration in CCS monitoring protocols.

How to cite: Li, T., Yu, T., Yu, N., Yang, Y., and Gu, Y. J.: Time-Lapse HVSR Analysis for Shallow Subsurface Monitoring at the CaMI.FRS CO2 Sequestration Site , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12093, https://doi.org/10.5194/egusphere-egu26-12093, 2026.

Underground mining induces seismicity and surface displacement. In Poland, in the Legnica Glogow Copper District near Wroclaw, induced earthquakes are particularly frequent with earthquakes of Mw3 and larger occurring many times a year. These earthquakes have shallow hypocentres of often less than 1 km and mostly above the mined copper layer.

The area around the mines also experiences a fast continuous surface subsidence of several millimeters per year caused by rock as well as groundwater extraction. This surface motion is observed through geodetic measurements on the ground and from space. The rate of surface motion is spatially very heterogeneous. Across wide areas above the active mining it even exceeds 10 mm/yr. Also sudden coseismic acceleration of surface motion is observed at the time of the larger earthquakes through space-borne InSAR. In these cases we often observe motion of several centimeters within a few days and with spatial extensions reaching a few kilometers.

Despite safety measures, the occurrence of some, also larger earthquakes is unexpected in space and time, which poses a particular threat to workers in the mines and but also to the subsurface mine structures as well as generally to the people, settlements and infrastructure above ground.

 

Our study investigates a number of larger events of the recent years by analyzing the locally recorded seismic waveforms jointly with measurements of the surface displacements based on InSAR and partly GNSS measurements. We aim to precisely locate the source processes of larger induced earthquakes and to characterize them as an interplay between shear-failure and collapse using full moment tensor models in a fully Bayesian inference framework. Potentially we can relate collapse and failure to the mining activities or other influences and improve our understanding of these unwanted events for mitigation measures.

The observations are best explained by large negative isotropic components accompanied by apparently significant shear failure mechanisms. Another finding is that our moment estimates systematically exceed the local catalog values. Challenges to be discussed are the impact of our single short-duration source model for possibly an accumulation of multiple events, possibly involving a larger volume and a longer duration, and the potential bias introduced by a simplified velocity model.

How to cite: Sudhaus, H., Witkowski, W., and Moser, S.: Investigating the source processes of underground-mining induced earthquakes based on geodetic and seismic observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12114, https://doi.org/10.5194/egusphere-egu26-12114, 2026.

EGU26-12236 | ECS | Posters on site | ERE5.1

Fault Network Activation During Controlled Hydraulic Stimulation Experiments in the BedrettoLab 

Martina Rosskopf, Anne Obermann, Antonio Pio Rinaldi, Kai Bröker, Linus Villiger, and Domenico Giardini

Understanding how faults are activated and earthquakes are triggered is still a central challenge in seismology and seismic hazard assessment. Controlled hydraulic stimulation experiments offer a valuable opportunity to study these processes under well-constrained conditions and at spatial and temporal resolutions that are rarely achievable in natural settings. In this study, we present the results of three hydraulic stimulations experiments conducted at the Bedretto Underground Laboratory and monitored by a dense, high-sensitivity seismic network.

These experiments revealed a complex spatio-temporal evolution of induced seismicity, characterized by the activation of a multi-segment fault network. Two dominant seismic clusters were activated early on and show a clear spatial connection to the injection borehole, suggesting that pore pressure is the main driver of seismicity within these clusters. At later stages, a third cluster with a different orientation was activated, despite showing no obvious direct hydraulic connection to the injection interval. Seismicity within this cluster occurred with a temporal delay compared to the other two clusters. This suggests that the fault activation was likely driven by indirect processes such as aseismic deformation, stress transfer, and delayed fluid migration.

The observed fault network activation closely resembles patterns commonly reported in natural earthquake sequences. These findings suggest that the physical mechanisms controlling fault reactivation and earthquake triggering are largely independent of scale, linking controlled field experiments and natural earthquakes. Our results emphasize the importance of fault network geometry and stress interactions in understanding induced and natural seismicity.

How to cite: Rosskopf, M., Obermann, A., Rinaldi, A. P., Bröker, K., Villiger, L., and Giardini, D.: Fault Network Activation During Controlled Hydraulic Stimulation Experiments in the BedrettoLab, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12236, https://doi.org/10.5194/egusphere-egu26-12236, 2026.

EGU26-12316 | ECS | Posters on site | ERE5.1

Frictional properties and fluid-induced reactivation of fault rocks from a granitic EGS reservoir 

Sangwoo Woo, Giuseppe Volpe, Luca Coppola, Cristiano Collettini, and Moon Son

In 2017, an MW 5.5 earthquake struck the Pohang region, representing the most damaging seismic event in South Korea, and has been linked in previous studies to hydraulic stimulation at the Pohang Enhanced Geothermal System (EGS) site. However, the relative roles of fluid injection, imposed stress state and fault-zone structure in nucleating this event remain a matter of debate, and the laboratory results presented here are intended to illuminate one mechanically plausible scenario rather than provide a unique causal explanation. Despite the scientific and societal importance of this earthquake, the frictional properties of rocks from the Pohang system are still poorly constrained. Here we experimentally characterize the frictional properties and slip behavior during fluid-induced reactivation of granodiorite wall rock powder and fault gouge recovered from the Pohang PX-2 borehole (~3.8 km depth). We first assessed the mineralogical assemblages of the two fault materials, which consist of mixtures of quartz, K-feldspar, plagioclase and phyllosilicates (mostly chlorite), with phyllosilicate contents varying between 15% and 23% for the wall rock and the fault gouge, respectively. We then measured friction, healing rate and the velocity dependence of friction for both materials under water-saturated conditions at normal stresses of 20–100 MPa using the BRAVA apparatus hosted at the National Institute of Geophysics and Volcanology (INGV). We performed frictional experiments in a double-direct-shear configuration, using a protocol consisting of a run-in at 10 µm/s, slide-hold-slide tests (SHS; hold times ranging between 3 and 3000 s), velocity-stepping tests (VS; velocities ranging between 0.3 and 300 μm/s), and fluid-injection tests (pore-pressure increases of 0.25 MPa every 5 min). Steady-state friction coefficients for both materials fall within the Byerlee range (μ ≈ 0.55–0.62). SHS tests reveal that both fault gouge and wall rock exhibit relatively high healing, with β in the range ≈ 0.0046–0.0092. Conversely, velocity-stepping tests reveal that, over the tested stress and velocity range, the wall rock has a slightly velocity-weakening to neutral behavior (a–b = −0.0007 to 0.0020), while fault gouge is predominantly velocity-neutral to strengthening (a–b = 0.0005 to 0.0028). Additional fluid-injection experiments indicate that, despite these slight differences in frictional properties, both the fault gouge and the wall rock can be reactivated under elevated pore pressure, with slip accelerating from creep to millimetre-per-second rates. Accompanying microstructural observations will examine whether differences in grain-size reduction, shear localization, or porosity evolution account for the similar reactivation behavior despite the slightly contrasting frictional properties. Overall, these measurements will help quantify how lithological heterogeneity, rate-and-state parameters, and pore-pressure evolution govern slip stability and the nucleation potential of injection-induced earthquakes in geothermal settings, with important implications for induced-seismicity hazard assessment in granitic EGS reservoirs.

How to cite: Woo, S., Volpe, G., Coppola, L., Collettini, C., and Son, M.: Frictional properties and fluid-induced reactivation of fault rocks from a granitic EGS reservoir, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12316, https://doi.org/10.5194/egusphere-egu26-12316, 2026.

EGU26-12815 | ECS | Posters on site | ERE5.1

Application of Data Science and Machine Learning Techniques for the Prediction of Induced Seismicity 

Leticia Raquel Garay Romero, Licia Faenza, Alex Garcia-Aristizabal, and Anna Maria Lombardi

The prediction of induced seismicity is a critical challenge for geological risk management and the safe operation of industrial facilities, such as geothermal projects. This study focuses on the Cooper Basin in Australia. We applied data science and machine learning techniques to analyze seismic time series, integrating two data sources: discrete seismological events (23,285 events) and continuous operational data sampled every 2 minutes (33,839 records).

The main objective was to develop machine learning models to predict, in future time windows of 10, 30, 60, and 90 minutes, two key variables: the number of seismic events or the maximum magnitude. The XGBoost and Random Forest algorithms were trained and compared. Model performance was evaluated using the , RMSE, and MAE metrics, and their interpretability was analyzed using SHapley Additive exPlanations (SHAP).

The results demonstrate that both models generate predictions consistent with the observations, showing better predictive performance in the longer time windows (60 and 90 minutes). This approach provides a valuable framework for the monitoring and proactive risk assessment of geothermal operations.

How to cite: Garay Romero, L. R., Faenza, L., Garcia-Aristizabal, A., and Lombardi, A. M.: Application of Data Science and Machine Learning Techniques for the Prediction of Induced Seismicity, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12815, https://doi.org/10.5194/egusphere-egu26-12815, 2026.

EGU26-13011 | Posters on site | ERE5.1

Enhancing Long-Term Seismic Analysis of Swiss Geothermal Projects through Waveform Similarity 

Tania Toledo, Verena Simon, Toni Kraft, and Tobias Diehl

Induced seismicity remains a significant challenge for the development of deep geothermal energy projects, with continued challenges at both the scientific and operational levels. 

Scientific level: Seismic monitoring at geothermal sites is commonly limited to periods of active operations such as hydraulic stimulation and testing, whereas datasets documenting the seismic response during shut-in and post-operational phases remain scarce. However, larger-magnitude earthquakes have been observed during shut-in phases, and in some cases months later, despite limited information on seismic activity during the active period. As a result, the processes governing delayed, larger-magnitude induced earthquakes remain poorly understood. 

Operational level: During active operations, the spatio-temporal evolution of induced seismicity provides one of the few direct indicators of subsurface processes. Real-time insight into whether seismicity evolves as expected or migrates toward potentially hazardous structures is essential for timely mitigation. Advanced Traffic Light Systems (ATLS) assess seismic hazard and risk based on observed seismic responses and rely on statistical and hydromechanical models to forecast the likelihood of induced events over the following hours to days. The reliability of these forecasts critically depends on the quality of the underlying earthquake catalog. Improved detection and location of small events and more robust magnitude estimates can substantially enhance hazard assessments and operational decision-making. 

To address these challenges, we introduce QuakeMatch (QM), a toolbox that leverages waveform similarity to improve seismic monitoring in both real-time and long-term applications. The workflow employs template matching based on events from a manually revised catalog, followed by refined magnitude estimation, event relocation of assembled events, and statistical analysis. 

We demonstrate the application of QM using the case studies from the Basel and Haute-Sorne deep geothermal projects. The Basel case is currently covered by earthquake catalogs with strongly varying location precision and completeness. A template-matched catalog by Herrmann et al. (2019), covering the period 2006–2019, does not include relocations and has not been updated since its publication. Here, QM is used to build a homogeneous long-term catalog of consistently high-precision earthquake locations that will improve our ability to assess the long-term response of this field over two decades up to the present day. For the Haute-Sorne case, we demonstrate the real-time application of QM, illustrating its potential to better inform advanced induced-seismicity-mitigation procedures (e.g., ATLS) with more reliable, consistent, and sensitive earthquake catalogs. Together, these examples illustrate the potential of combining long-term catalog enhancement with real-time monitoring to support safer and more informed geothermal operations. 

How to cite: Toledo, T., Simon, V., Kraft, T., and Diehl, T.: Enhancing Long-Term Seismic Analysis of Swiss Geothermal Projects through Waveform Similarity, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13011, https://doi.org/10.5194/egusphere-egu26-13011, 2026.

EGU26-13423 | ECS | Orals | ERE5.1 | ERE Division Outstanding ECS Award Lecture

Understanding fluid injection-induced earthquakes: From causal mechanisms to fault frictional slip 

Wenzhuo Cao

The global energy transition increasingly relies on the sustainable use of the subsurface, which commonly involves fluid injection. Such injection can induce earthquakes, posing significant challenges to the safety and operability of geo-energy applications. Addressing these challenges requires a geomechanical understanding of induced seismicity and the coupled subsurface processes that govern it. This Award Lecture introduces recent research on fluid injection-induced earthquakes, spanning the evaluation of causal mechanisms to an in-depth understanding of the fault-slip processes that control earthquake magnitude and frequency.

The first part of the presentation focuses on identifying and evaluating the causal mechanisms for injection-induced earthquakes. The problem is formulated as assessing the susceptibility of fracture and fault slip driven by coupled thermo-hydro-mechanical (THM) processes in fractured porous media. Through several geo-energy case studies, it is demonstrated that induced seismicity commonly results from fracture and fault reactivation through multiple, co-occurring mechanisms. The relative contribution of these mechanisms largely depends on regional geology, fracture and fault properties, ambient stress conditions, and operational parameters. Fluid overpressure typically develops rapidly following injection and may influence a large area, depending on hydraulic connectivity and fault permeability. Poroelastic stressing accompanies fluid pressurisation, with its contributions controlled by the distance to susceptible faults and fault orientation relative to the ambient stress field. Thermal stressing is generally more spatially localised around injection wells but can become dominant over longer timescales. In addition, fault slip-induced stress transfer can explain seismicity beyond the region affected by fluid pressure and poroelastic stress changes. Understanding these mechanisms enables the development of physics-based approaches for induced seismicity hazard assessment that explicitly account for both geological conditions and operational strategies.

The second part of the presentation addresses fault frictional slip processes that ultimately control the earthquake magnitude and frequency. Three key governing processes are identified for injection-induced fault slip: fluid pressurisation, hydraulic diffusion, and frictional nucleation, each characterised by a distinct timescale. Their interactions give rise to a wide range of induced earthquake behaviours. To disentangle their combined effects, a coupled hydro-mechanical-frictional modelling framework was developed that integrates frictional contact models for faults with poroelastic models for surrounding rocks. The results have shown that frictional properties exert first-order control on fault slip regimes and the maximum earthquake magnitude, whilst fluid pressurisation primarily governs earthquake frequency and also influences the maximum magnitude through poroelastic stressing. These effects are further modulated by hydraulic diffusion, highlighting the role of reservoir hydraulic conductivity in controlling how injected fluids interact with distant faults. Building upon this understanding, this contribution illustrates how fluid pressurisation rate influences induced earthquake magnitude and frequency, and discusses the implications for designing injection strategies that minimise seismic risk while maintaining operational efficiency.

Acknowledgement: I gratefully acknowledge the support and nomination by Prof. Sevket Durucan, Dr. Suzanne Hangx, Prof. Chris Spiers, Prof. Paul Glover, and Prof. Keita Yoshioka, and the many collaborators who contributed to the research presented.

How to cite: Cao, W.: Understanding fluid injection-induced earthquakes: From causal mechanisms to fault frictional slip, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13423, https://doi.org/10.5194/egusphere-egu26-13423, 2026.

EGU26-14235 | ECS | Orals | ERE5.1

Signatures of flow path creation in isotropic components of microseismic moment tensors at Utah FORGE 

Peter Niemz, Gesa Petersen, Jim Rutledge, Katherine Whidden, and Kris Pankow

The Utah Frontier Observatory for Research in Geothermal Energy (FORGE) is a field-scale laboratory for the study of enhanced geothermal systems (EGS) in low-permeable granitic and metamorphic basement rocks. Utah FORGE comprises a highly deviated injection–production well pair reaching a depth of ~2.5km and temperatures above 220°C. The site is monitored by multiple comprehensive microseismic networks with sensors installed at the surface, in shallow boreholes, and in deep boreholes at reservoir level. Following high-pressure hydraulic stimulation campaigns in 2022 and 2024, the wells were successfully connected through at least two principal fracture zones.

We study the induced microseismicity and its relation to flow path creation processes by performing waveform-based full moment tensor (MT) inversions for >180 events (local magnitude ML 0.0–1.9) recorded during the 2024 stimulations. Including non–double–couple (non-DC) or, more specifically, isotropic components helps characterize a complex reservoir development. Locally, most events exhibit highly similar strike-slip mechanisms consistent with the regional stress field, though minor rotations are observed between different fractured zones. We interpret well-resolved positive isotropic components as indicators for tensile opening components in the microseismic events. The maximum isotropic component increases with cumulative injected volume. Interestingly, the tensile components are more pronounced in areas dominated by fault reactivation compared to zones characterized by the opening of new hydraulic fractures and fracture networks. Our analysis highlights the complex interplay between the hydraulic activation of pre-existing fractures and the hydraulic opening of newly formed macrofractures during the stimulations at Utah FORGE. While resolving microseismic non-DC components requires a thorough, challenging analysis of resolution and uncertainties, their inclusion in routine monitoring can help illuminate not only where the reservoir is breaking but also how the hydraulic connection is established.

How to cite: Niemz, P., Petersen, G., Rutledge, J., Whidden, K., and Pankow, K.: Signatures of flow path creation in isotropic components of microseismic moment tensors at Utah FORGE, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14235, https://doi.org/10.5194/egusphere-egu26-14235, 2026.

EGU26-14295 | ECS | Posters on site | ERE5.1

Investigating the Correlation Between Post-Injection Trailing Seismicity and Wellhead Pressure Decay in Enhanced Geothermal Systems 

Riccardo Minetto, Zhiwei Wang, Olivier Lengliné, and Jean Schmittbuhl

Injection of fluids during reservoir stimulation aims to enhance reservoir permeability but induces seismic activity that persists for several hours to several months after injection has ceased. Physical and hybrid models have been successfully applied to reproduce and forecast observed seismicity rates during and after injection. However, these models are typically site-dependent, raising the question of whether a general relationship between pressure and seismicity decay can be observed across different sites and operations.

In this study, we investigate the correlation between post-injection pore pressure decay and the decrease in seismicity rate using data from multiple EGS injection operations that share similar properties. First, the performance of several empirical statistical models is evaluated to describe the decrease in seismicity rate. Second, wellhead pressure decay is shown to be best described by a simple exponential model. Lastly, we introduce a time-to-fraction metric to compare the pressure and seismicity evolution after shut-in. We show that the times required to reach a given fraction of the initial rate for both pressure and seismicity are correlated, with pressure evolution being slower than seismicity rate evolution. No correlation is observed between seismicity decay and injection parameters such as injected volume, average injection pressure, or injection duration. These observations suggest that pore pressure has a limited influence on seismicity decay, which has strong implications for reservoir management.

How to cite: Minetto, R., Wang, Z., Lengliné, O., and Schmittbuhl, J.: Investigating the Correlation Between Post-Injection Trailing Seismicity and Wellhead Pressure Decay in Enhanced Geothermal Systems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14295, https://doi.org/10.5194/egusphere-egu26-14295, 2026.

EGU26-14814 | Orals | ERE5.1

Micro-seismicity in the Hverahlíð high-temperature geothermal field, Hengill, SW-Iceland 

Thorbjörg Ágústsdóttir, Ásdís Benediktsdóttir, Egill Árni Gudnason, Rögnvaldur Líndal Magnússon, Sæunn Halldórsdóttir, Gudni Axelsson, Helga Margrét Helgadóttir, and Sveinborg H. Gunnarsdóttir

The Hverahlíð high-temperature geothermal field is located in the southern part of the Hengill volcanic complex in southwest Iceland. Prior to the onset of geothermal production in 2016, seismic activity in the area was limited. Since then, persistent micro-seismicity has been detected, characterised by a diffuse spatial pattern and only minor swarm activity. Despite covering just ~2 km², Hverahlíð hosts some of Iceland’s most productive geothermal wells, with measured temperature exceeding 300°C at around 1.5 km depth.

In this study, we analyse seismicity in Hverahlíð from 2016 to 2025, recorded by a varying number of seismometers (14 to 40) deployed across the wider Hengill area. The core network consists of permanent stations operated by Iceland GeoSurvey (ÍSOR) for ON Power, supplemented by the regional SIL-network of the Icelandic Meteorological Office. Additionally, 30 temporary stations were installed during the COSEISMIQ project (2018–2021), significantly improving the local detection capability and spatial resolution.

Seismicity in Hverahlíð is dominantly micro-seismicity, with ~90% of the activity of ML < 1.0, and a magnitude range of ML -0.3 to 3.5. High-resolution relative relocations show that seismicity is confined to 2-3.5 km depth below sea level, i.e., located slightly below the bottom of the production wells and organised in one main cluster and another significantly smaller cluster, both trending NNE-SSW within the production area.

Although the Hverahlíð area is highly fractured with cross-cutting faults trending from NNE-SSW to ENE-WSW, the observed seismicity does not directly illuminate known surface faults. Instead, the earthquake distribution reflects the geothermal production zone, closely matching the geometry of the geothermal system as inferred from existing resistivity models. The earthquake depth distribution may reflect, at least partially, cooling and thermal contraction of the hot host rock induced by deep fluid convection linked to the heat source of the geothermal system. Comparison with other high-temperature geothermal systems in Iceland suggests that the seismicity may delineate the base of a highly permeable convective geothermal reservoir.

Despite considerable production driven pressure draw-down in Hverahlíð, only around 18% of earthquake source mechanisms show pure normal faulting, whereas 55% show pure strike-slip faulting. As the production area will grow in lateral extent in coming years through planned step-out-wells, a corresponding increase in the lateral extent of seismicity is possible.

How to cite: Ágústsdóttir, T., Benediktsdóttir, Á., Gudnason, E. Á., Magnússon, R. L., Halldórsdóttir, S., Axelsson, G., Helgadóttir, H. M., and Gunnarsdóttir, S. H.: Micro-seismicity in the Hverahlíð high-temperature geothermal field, Hengill, SW-Iceland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14814, https://doi.org/10.5194/egusphere-egu26-14814, 2026.

The injection of produced water back into producing permeable formations is regarded to be of low risk of inducing earthquakes because injection into producing conventional reservoirs generally does not lead to a net increase in reservoir pressure. The rise of production from tight unconventional reservoirs, on the other hand, required injection into non-producing aquifers. While unsurprising in hindsight, the concomitant increase in induced seismicity was unexpected based on the assumption, later shown to be false, that faults in stable cratonic sedimentary basins such as those in Texas and Oklahoma are not critically stressed. Complicating matters more, seismicity preferentially occurred in crystalline basement well below the injection target. Geomechanical models demonstrate that this response can be attributed to poroelastic stresses that are active over a larger distance and greater depth than the direct pore pressure disturbance. Our fully coupled poroelastic finite element simulations also demonstrated that in basins of large-volume injection, stress changes cannot be attributed to a single well or injection operation but reflect the cumulative effect of multiple disposal and production wells on a regional scale, making mitigation significantly more challenging. The difficulty of hindcasting observed seismic events on known and well-instrumented faults also demonstrated that effective forecasting of a seismic response would be difficult. This presentation will discuss viable approaches to mitigating the induced seismicity risk, concluding that active pressure management and avoiding injection in close vicinity to known large faults or close to infrastructure are perhaps the most effective approaches for mitigating earthquake risk associated with large-volume injection of wastewater and CO2 into aquifers.

How to cite: Eichhubl, P., Haddad, M., and Bump, A.: The geomechanics of induced seismicity associated with large-volume fluid injection—implications for risk mitigation , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15038, https://doi.org/10.5194/egusphere-egu26-15038, 2026.

EGU26-16611 | ECS | Posters on site | ERE5.1

Stress perturbations and fault reactivation during cold fluid Injection - impact of hydraulic anisotropy  

Tatia Sharia, Birgit Müller, and Andreas Rietbrock

Cold fluid injection into a hot subsurface reservoir alters the in situ temperature, pore pressure, and stress fields through multiple interacting physical mechanisms. Poroelastic stress changes arise from pressure diffusion, whereas thermomechanical stresses are driven by reservoir cooling and associated thermal contraction. In this study, we investigate how hydraulic anisotropy in the reservoir controls the spatio-temporal evolution of these stress perturbations and related failure potential. We present results from fully coupled thermo-hydro-mechanical (THM) simulations using a three-dimensional reservoir-scale generic model, considering different injection scenarios, including single injection wells and doublets, as well as isotropic and anisotropic hydraulic properties. In general, both temperature and pore pressure variations affect the radial and tangential stress components relative to the injection site in distinct ways, even under isotropic material conditions. This distinction is critical for evaluating slip tendency and calculating Coulomb failure stress changes (ΔCFS) for the faults in the vicinity of the injection well. For anisotropic reservoir conditions, we compare the temporal evolution of pore pressure and temperature during single-well injection against isotropic reference cases and assess the implications for ΔCFS. For 20 years of continuous injection and permeability anisotropy factor of 10, the temperature front propagates approximately 20 times faster along the high-permeability direction. While the rate of pressure diffusion scales with the permeability component in the direction of propagation, the resulting pressure magnitude is governed by permeability components in the perpendicular directions. Similarly, thermally induced stresses evolve more rapidly in high-permeability directions and more slowly in low-permeability directions, as well as producing different magnitude changes in radial and tangential stress components. The modeled ΔCFS indicates that although fault orientation influences the calculated stress changes, the dominant control arises from directional fluid flow associated with hydraulic anisotropy. In conclusion, hydraulic anisotropy exerts a first-order control on the spatial and temporal distribution of pressure and temperature perturbations, leading to pronounced directional variations in induced stress fields and the corresponding Coulomb failure stress evolution in the vicinity of geothermal boreholes. These results provide a basis for optimized drill site selection and well orientation strategies aimed at minimizing fault reactivation and reducing the risk of injection-induced seismicity. 

 

How to cite: Sharia, T., Müller, B., and Rietbrock, A.: Stress perturbations and fault reactivation during cold fluid Injection - impact of hydraulic anisotropy , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16611, https://doi.org/10.5194/egusphere-egu26-16611, 2026.

EGU26-17447 | ECS | Posters on site | ERE5.1

Understanding the Non-Stationary Nature of Human-Induced Earthquakes and its Impact on Geothermal Energy Production 

Lada Dvornik, Annemarie Muntendam-Bos, Jan Dirk Jansen, and Loes Buijze

Anthropogenic activity in the subsurface causes stress perturbations which can lead to the onset of seismicity. One of the notorious examples is the Groningen gas field in the northeast part of the Netherlands which is among the largest in Europe. Hydrocarbons have been produced there since 1963 until the field’s ultimate shutdown in October 2023. From December 1991 until January 1st, 2026, total of 1561 events have been recorded in this area, with magnitude ranging from  to . The  events caused extensive damage to buildings and quite a societal unrest as well as scepticism towards subsurface operations in general. Considering, it is crucial to identify an envelope for safe utilization of the subsurface to be able to continue its usage for energy transition while limiting the risk of induced seismicity.

To be able to limit the risk of seismicity from subsurface operations, it is necessary to understand the non-stationary nature of induced seismicity, meaning the underlying physical causes of the observed spatial and temporal variations in event locations and frequency-magnitude distribution. This research is based on the hypothesis that the fault spatial distribution and geometry (dip angle, offset) in conjunction with operational parameters (pressure history, rates, injection temperatures) are the causal processes of the temporal and spatial variations in the Gutenberg-Richter parameters.

I will present the results from modelling production induced seismicity using the Groningen field as a study area. The results include synthetic earthquake catalogues obtained by modelling the event nucleation and magnitudes using a semi-analytical approach of slip weakening faults. For this model, fault geometry and pressure history serve as input. In order to obtain multiple catalogues spanning the full range of uncertainty, a Monte Carlo sensitivity analysis is conducted for different reservoir and fault properties. Subsequently, several statistical comparison tests of the simulated catalogue with the observed seismicity allows us to derive posterior estimates for our properties and provide crucial insight into how we are doing solving the puzzle of what is causing the observed spatiotemporal behaviour of induced earthquakes.

How to cite: Dvornik, L., Muntendam-Bos, A., Jansen, J. D., and Buijze, L.: Understanding the Non-Stationary Nature of Human-Induced Earthquakes and its Impact on Geothermal Energy Production, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17447, https://doi.org/10.5194/egusphere-egu26-17447, 2026.

EGU26-17827 | ECS | Posters on site | ERE5.1

3D Modeling of fluid-induced seismicity on fault with heterogeneous frictional asperities 

Jiayi Ye, Zhenhuan Wang, Federico Ciardo, Antonio Pio Rinaldi, Luca Dal Zilio, and Domenico Giardini

A key challenge in induced seismicity is that fluid injection perturbs stress and pore pressure on faults with heterogeneous properties, leading to complex earthquake nucleation, migration and magnitude. The BedrettoLab (Bedretto Underground Laboratory for Geosciences and Geoenergies), located in the Swiss Alps, provides a unique natural testbed to study how these coupled hydro-mechanical processes interact with fault heterogeneity under controlled injection conditions, with direct access to well-characterized and densely instrumented fault zones. Previous characterization of the target MC fault zone at BedrettoLab show that layers of frictional velocity-strengthening (VS) fault gouge are embedded within velocity-weakening (VW) granitic bare rock, forming a strongly heterogeneous frictional architecture. However, how this frictional partitioning controls fault slip behavior and the magnitude of induced seismicity remains unclear. In this study, we use the newly developed 3D hydro-mechanical model HydroMech3D to explore the interplay between frictional heterogeneity and seismicity in fluid injection simulations, governed by rate- and state-dependent friction. We simulate injection scenarios using parameters and conditions derived from the ongoing FEAR (Fault Activation and Earthquake Rupture) experiments at Bedretto. Our simulations investigate how the spatial distribution of VS and VW patches control seismicity magnitude. By systematically changing the partition of VS and VW patches, we explore its influence on event size distributions and maximum magnitudes. Further simulations are conducted under various hydro-mechanical pre-conditioning conditions, by pre-determining the pressurized patch on the fault via the injection protocol prior to the main injection. These simulations allow us to understand whether fault pre-conditioning may influence the maximum magnitude of induced seismicity. Our results emphasize the critical role of frictional heterogeneity and injection strategy in fault dynamics, providing new insights into the hydro-mechanical behavior of complex fault zones during fluid injection and improving seismic risk assessment and mitigation strategies.

How to cite: Ye, J., Wang, Z., Ciardo, F., Rinaldi, A. P., Dal Zilio, L., and Giardini, D.: 3D Modeling of fluid-induced seismicity on fault with heterogeneous frictional asperities, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17827, https://doi.org/10.5194/egusphere-egu26-17827, 2026.

EGU26-17977 | Posters on site | ERE5.1

A Hybrid Implicit–Explicit XFEM Framework for Fully Coupled Hydro-Mechanical Dynamic Simulation of Injection-Induced Seismicity 

Mohammad Sabah, Mauro Cacace, Hannes Hofmann, Guido Blöcher, Mohammad Reza Jalali, and Iman R. Kivi

Accurate simulation of injection-induced seismicity requires to solve for strongly coupled hydro-mechanical physics describing processes acting over widely separated spatiotemporal scales, ranging from reservoir scale fluid diffusion to fault nucleation and rapid dynamic rupture. In this study, we present a monolithic hydro-mechanical dynamic framework based on the extended finite element method (XFEM) for modeling fluid-induced fault reactivation governed by rate-and-state friction. Faults are represented as embedded displacement discontinuities within a poroviscoelastic medium, enabling a consistent treatment of fault slip, unilateral contact constraints, stress-dependent permeability evolution, and fluid exchange between the fault and the surrounding porous matrix.

To overcome the computational cost associated with fully implicit time integration, we develop a hybrid implicit–explicit (IMEX) time-integration strategy. The implicit solver is employed during the quasi-static and nucleation phase, while an explicit scheme is activated only during the coseismic stage, once a prescribed slip-velocity threshold is exceeded. This adaptive solver switching allows accurate resolution of the dynamic rupture with substantial reduction of the computational effort. The approach is combined with adaptive time stepping to efficiently capture both slow interseismic evolution and fast seismic transients within a unified framework.

Numerical simulations of fluid injection into a faulted reservoir demonstrate that, despite unconditional stability, fully implicit schemes require minimum time steps comparable to the Courant–Friedrichs–Lewy limit to accurately resolve rupture nucleation and propagation. In contrast, the proposed IMEX formulation can reproduce fault slip evolution, stress redistribution, frictional weakening, seismic moment, and event magnitude with high fidelity, while reducing computational cost by approximately 60–77% relative to fully implicit simulations. Differences between the two approaches are primarily limited to peak slip velocities and rupture speeds, whereas rupture timing, accumulated slip and event-scale seismic metrics remain consistent.

The proposed XFEM-based IMEX framework provides a robust and computationally efficient tool for simulating injection-induced seismicity, offering a practical pathway toward reservoir scale simulations of coupled fault–fluid systems relevant to geo-energy applications and seismic hazard assessment.

How to cite: Sabah, M., Cacace, M., Hofmann, H., Blöcher, G., Reza Jalali, M., and R. Kivi, I.: A Hybrid Implicit–Explicit XFEM Framework for Fully Coupled Hydro-Mechanical Dynamic Simulation of Injection-Induced Seismicity, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17977, https://doi.org/10.5194/egusphere-egu26-17977, 2026.

Mining districts in Chile are located within one of the most seismically active tectonic environments on Earth, which makes it challenging to distinguish between natural crustal seismicity and seismicity potentially influenced by mining. A key open question is whether large-scale mining operations produce a measurable and spatially coherent statistical signature in the surrounding shallow crust. In this study, we evaluate this hypothesis using the Gutenberg–Richter b-value as a quantitative proxy for local stress conditions and the degree of rock mass damage and fracturing. We focus on the seismic environment surrounding major mining districts in Chile, restricting the analysis to shallow crustal events with depths shallower than 10 km. This depth filter aims to isolate the seismic response of the upper crust that is most likely to be affected by mining-related stress perturbations, while reducing the contribution of deeper subduction-driven tectonic seismicity. To resolve spatial variations at kilometer scale, we implement a high-resolution concentric-ring analysis centered on each mining district, using 1 km radial bins extending outward from the extraction centers. To ensure statistical robustness and comparability across sites, the magnitude of completeness (Mc) is estimated dynamically using the maximum curvature method, yielding reference values close to ML ≈ 1.87 for the analyzed catalog. The Gutenberg–Richter b-value is then computed using the Aki–Utsu maximum-likelihood estimator, providing a rigorous and stable framework for inter-site comparisons under contrasting geomechanical and operational settings. The analysis reveals clear and systematic differences depending on the mining method. Underground mining environments show a pronounced increase in b-value (b > 1.5) within the first ~5 km, consistent with elevated rates of microseismicity and enhanced brittle damage associated with caving-related processes. In contrast, open-pit operations exhibit a comparatively stable b-value pattern with lower spatial dispersion. In both settings, b-values progressively converge toward the regional tectonic reference level (b ≈ 1.0) with increasing distance from the extraction centers, suggesting a characteristic radius of direct mining influence on the order of ~15–20 km. These preliminary results show that kilometer-scale mapping of the Gutenberg–Richter b-value provides a sensitive and interpretable metric to quantify the spatial footprint of mining-related seismic perturbations in the shallow crust. The observed b-value gradients offer a practical tool for regional-scale geomechanical monitoring, supporting the discrimination between background tectonic seismicity and elastic stress changes induced by excavation and/or large-volume rock mass caving in Chilean mining districts.

How to cite: Roquer, T. and Ravest, B.: Mining-Related b-Value Anomalies in the Upper Crust: A High-Resolution Ring Analysis Across Chilean Mining Districts , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20770, https://doi.org/10.5194/egusphere-egu26-20770, 2026.

EGU26-21070 | ECS | Orals | ERE5.1

Network Performance Evaluation workflow and test for seismic monitoring of geothermal projects in Switzerland 

Verónica Antunes, Verena Simon, Tania Toledo, and Toni Kraft
Switzerland is investing in geothermal energy solutions to decrease CO2 emissions by 2050. However, geothermal energy exploration can carry the risk of induced seismicity. Adequately managing seismic risk is key to establishing safe and economically viable geothermal projects. To monitor possible induced seismicity, dedicated seismic networks in the vicinity of the monitored projects have to be in place. These networks must be sensitive enough to follow the evolution of the microseismicity and allow the operators to run traffic-light systems and take actions before larger events occur. Current geothermal guidelines establish the minimum monitoring requirements of such networks, providing specific values for Magnitude of Completeness (Mc) and location accuracies.
To adequately monitor geothermal projects in Switzerland, we developed a workflow that goes from network geometry planning to its final installation (Antunes et al., 2025). This workflow includes network performance and evaluation procedures in order to ensure the minimum monitoring requirements proposed in the Good Practice Guide for managing induced seismicity in Switzerland (Kraft et al., 2025). To evaluate beforehand the detection sensitivity of a seismic network, we estimate the Bayesian Magnitude of Completeness (BMC), optimised for Switzerland. We additionally estimate the theoretical location uncertainties inside the network by generating and locating a synthetic catalogue of events, using the 3D velocity model for Switzerland. Both approaches consider the background noise level at the stations and the specific network geometry.
In December 2017, a seismic network was installed to monitor the geothermal activities of the AGEPP project in Lavey-les-Bains, Switzerland. This seismic network was in operation until mid 2023, acquiring the natural seismicity of this active alpine area. We use the public seismic catalogue as input for a template matching (QuakeMatch, Toledo et al., 2024) scan to increase the sensitivity, reducing the initial Mc by 2 orders of magnitude. We evaluate and test the network performance tools of our workflow by comparing the results of our numerical estimations with the resulting seismic catalogues (Mc and location errors). Our results show good agreement between the theoretical methods' estimations and the catalogue data registered with the network, proving that our numerical tools are a good approach to estimate the performance of a network when no earthquake information is available, e.g., right after a network installation.
 
References:
Antunes, V., Kraft, T., Toledo Zambrano, T. A., Reyes, C. G., Megies, T., & Wiemer, S. (2025). Optimising Seismic Networks for Enhanced Monitoring of Deep Geothermal Projects in Switzerland. In Proceedings of the European Geothermal Congress 2025. European Geothermal Energy Council. https://doi.org/10.3929/ethz-c-000791611
Kraft, T., Roth, P., Ritz, V., Antunes, V., Toledo Zambrano, T. A., & Wiemer, S. (2025). Good-Practice Guide for Managing Induced Seismicity in Deep Geothermal Energy Projects in Switzerland. ETH Zurich. https://doi.org/10.3929/ethz-b-000714220
Toledo, T., Simon, V., Kraft, T., Antunes, V., Herrmann, M., Diehl, T., & Villiger, L. (2024). The QuakeMatch Toolbox: Using waveform similarity to enhance the analysis of microearthquake sequences at Swiss geothermal projects (No. EGU24-13824). Copernicus Meetings. https:.//doi.org/10.5194/egusphere-egu24-13824

How to cite: Antunes, V., Simon, V., Toledo, T., and Kraft, T.: Network Performance Evaluation workflow and test for seismic monitoring of geothermal projects in Switzerland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21070, https://doi.org/10.5194/egusphere-egu26-21070, 2026.

EGU26-124 | Posters on site | ERE5.2

Abrupt structural deformation changes from the boundary to the interior of the Craton Basin 

Lei Huang, Zhao Wang, Yiyong Zhang, Xin Li, and Chiyang Liu

Stable intraplate cratonic blocks usually have less structural deformation and fewer earthquakes than other locations on Earth, but with strong compressional deformation around their periphery. Investigating how and why this different deformation occurred is beneficial for understanding why the cratonic block is so stable and how the intraplate in-plane stress is transmitted. In this work, we first investigated the structural deformation changes from the margin to the interior of the western Ordos Block (OB; one of the most tectonically stable area in China) via seismic data. The results show abrupt structural deformation changes from the margin to the interior of the OB in terms of the deformation strength (from strong to weak), structural orientation (high angle oblique relationships), and kinematics (from compression to wrenching). Our investigation also shows that such phenomena are widespread in cratonic blocks worldwide. The abrupt changes are probably induced by special in-plane stress transfer inside the cratonic block: when far-field stress is transmitted into continental interiors from active plate margins, the weak belt around the cratonic block filters and accommodates the in-plane stress. Consequently, this decreases the stress, changes the stress direction, and transmits the in-plane stress along a shallower layer (probably less than 1500 m). Furthermore, the compression stress from the plate margin is converted into shear stress within the cratonic block. This stress transmission manner makes reactivation of the deep preexisting faults difficult under far-field horizontal plate-boundary stresses in the cratonic block without vertical forces from the mantle, guaranteeing long-term stability and low seismicity. This understanding can provide a new perspective for the interpretation of earthquakes in stable continental regions. It can also be applied to appraise the long-term stability of sites for the storage of CO2.

How to cite: Huang, L., Wang, Z., Zhang, Y., Li, X., and Liu, C.: Abrupt structural deformation changes from the boundary to the interior of the Craton Basin, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-124, https://doi.org/10.5194/egusphere-egu26-124, 2026.

Abstract: Accurate construction of multi-scale fracture models is essential for optimizing hydraulic fracturing design, predicting sweet-spot distribution, and improving shale gas recovery in deep, structurally complex reservoirs. The Wufeng–Longmaxi shale in the northern Luzhou area is characterized by strong tectonic deformation, lithological heterogeneity, and fracture development across multiple scales. To address these challenges, this study proposes an integrated multi-scale fracture modeling framework that couples reservoir geomechanics, multi-attribute seismic analysis, and microstructural characterization. First, pre-stack seismic inversion was performed to derive elastic parameters, including P-impedance, Vp/Vs ratio, and density, which were further used to construct 3D mechanical property volumes such as brittleness index, Young’s modulus, and Poisson’s ratio. Curvature attributes and ant-tracking analysis were applied to delineate zones of enhanced structural deformation and large-scale fracture corridors. Second, triaxial rock mechanics experiments and CT-based digital core analysis were conducted to calibrate lithology-dependent failure criteria and layer-parallel anisotropic mechanical parameters for siliceous and calcareous shales, forming the basis of a heterogeneous geomechanical model. Finite-element simulations were then used to resolve the present-day in-situ stress field and quantify fracture openness, density, and orientation under mechanical–stratigraphic constraints. Results show that: (1) a NW–SE trending high-curvature anticline dominates the northeastern study area, where brittle siliceous shale (brittleness index > 0.65) accounts for 58%, and the maximum horizontal stress (NW 130°–150°) provides favorable conditions for fracture development; (2) large-scale fractures (>10 m) are controlled by curvature ridges and fault transfer zones, while mesoscale fractures (1–10 m) correlate positively with the product of brittleness index and bedding density, and (3) microscale fractures (<1 mm) exhibit strong coupling with TOC-rich domains (TOC > 3.5%). Integrating curvature volumes, ant-tracking results, geomechanical simulations, and microfracture fractal parameters yields a hierarchical workflow linking macroscopic structural guidance, mesoscale mechanical response, and microscale pore–fracture attributes. Field validation shows that the predicted fracture-rich zones match production performance with an accuracy of 82%. The L202 well, deployed using this workflow, achieved a post-fracturing daily gas rate of 2.3×10⁵ m³, 37% higher than adjacent wells. This integrated methodology overcomes the limitations of single-scale modeling and provides a robust framework for 3D shale gas reservoir evaluation and development in complex structural domains.

Keywords: Multi-scale fracture modeling; reservoir geomechanics; seismic attribute integration; in-situ stress; Luzhou area

How to cite: Ren, Q.: A Multi-Scale Fracture Modeling Framework Driven by Integrated Reservoir Geomechanics and Seismic Attribute Analysis: A Case Study from the Northern Luzhou Shale Gas Play, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1485, https://doi.org/10.5194/egusphere-egu26-1485, 2026.

EGU26-2105 | ECS | Posters on site | ERE5.2

Fracture modeling of the hydrocarbon reservoir using geostatistical and neural network methods in the SW Iran Oilfield  

Zahra Tajmir Riahi, Ali Faghih, Bahman Soleimany, Khalil Sarkarinejad, and Gholam Reza Payrovian

Abstract

Fracture characterization and modeling are essential for hydrocarbon exploration and enhanced production. To model the fracture network in the Asmari reservoir of the Rag-e-Sefid Oilfield (SW Iran), this research characterizes fracture intensity using well, fracture driver, and fracture controller data. First, these data are analyzed to estimate fracture intensity. Then, fracture intensity is modeled using geostatistical methods. The geostatistical outputs are compared and calibrated based on the structural setting of the study area and the fracture indicator. Finally, selected fracture intensity data are integrated into a single model using an artificial neural network, resulting in a comprehensive fracture intensity model for the Asmari reservoir of the Rag-e-Sefid Oilfield. The results show that fracture intensity increases near the Rag-e-Sefid and Nourooz-Hendijan-Izeh Faults and in the fold forelimb and crest. The highest fracture intensity in the Asmari reservoir is observed at the intersection of structures with the N-S Arabian trend and the NW-SE Zagros trend, where the fold axis has rotated. Generally, the northwestern part of the Rag-e-Sefid anticline has higher fracture intensity than the southeastern part. The high fracture intensity in the northwest part of the Rag-e-Sefid Oilfield is related to inversion tectonics, multi-stage reactivation along pre-existing basement structures, and an older deformation history in this area compared to its southeastern part. The Asmari reservoir in the NW part of the Rag-e-Sefid anticline contains a greater share of oil and gas in its hydrocarbon traps than the SE part. Moreover, the results of this study indicate that the simultaneous use of different data and the integration of geostatistical and artificial neural network methods can effectively predict fracture distribution in hydrocarbon reservoirs and be used as a suitable technique for fracture modeling in natural oil and gas fields. This research suggests that artificial intelligence and quantum computing techniques provide efficient solutions for characterizing and modeling the entire scale of geological fractures in hydrocarbon reservoirs.

Keywords: Fracture modeling, Geostatistical and neural network methods, Asmari reservoir, Rag-e-Sefid Oilfield, SW Iran

How to cite: Tajmir Riahi, Z., Faghih, A., Soleimany, B., Sarkarinejad, K., and Payrovian, G. R.: Fracture modeling of the hydrocarbon reservoir using geostatistical and neural network methods in the SW Iran Oilfield , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2105, https://doi.org/10.5194/egusphere-egu26-2105, 2026.

EGU26-3278 | ECS | Posters on site | ERE5.2

Integrated Characterization of Fracture Orientations and Hydraulic Properties in Crystalline Bedrock 

Hande Okutan, Jon Engström, Daniel Carbajal-Martinez, Mira Markovaara-Koivisto, Rebekka Salmi, Heini Reijonen, and Evgenii Kortunov

Understanding hydraulic properties in fractured crystalline bedrock is essential for predicting groundwater flow and heat transport in deep geological settings. This study focuses on the Kopparnäs Test Site in southern Finland, where the bedrock mainly consists of granites, granodiorites, and, commonly migmatitic mica gneiss.

Fracture orientation and aperture were characterized using acoustic (ABI) and optical borehole imaging (OBI), combined with hydraulic conductivity measurements obtained from zone-based slug tests in a borehole drilled to a depth of 233 m. Seven test zones at depths ranging from 18 m to 132 m were selected for integrated hydraulic conductivity and fracture analysis. The borehole intersects a nearly vertical east–west striking fault zone at approximately 100 m depth, where three core zones were targeted for hydraulic conductivity measurements. Each zone was analysed in terms of fracture frequency, orientation, and infilling to achieve an integrated understanding of hydraulic behaviour.

Structural analysis indicates that most fractures are steeply dipping, with dominant NNE-SSW orientations and dips towards the SSE. Sub-horizontal fractures mainly occur at shallow depths within the upper 100 m, which is typical of Finnish crystalline bedrock due to glacial unloading after the latest glaciation. Between 100-130 m, the borehole intersects a sub-vertical fault zone that significantly increases fracture frequency. Below this zone fracture frequency decreases markedly with only sporadic fractures observed.

Hydraulic conductivity remains within the same order of magnitude (10-9 m/s) but varies between zones reflecting differences in fracture characteristics rather than fracture density alone. Higher hydraulic conductivity is observed at shallow depths where fractures are predominantly sub-horizontal and partially open. In contrast, deeper sections are dominated by steeply dipping, mineral-filled fractures associated with reduced conductivity. Intermediate conductivities reflect mixed orientations and aperture conditions. Overall, fracture orientation and infilling exert a stronger control on hydraulic conductivity than fracture frequency, the role of fracture connectivity, aperture and mineral filling in governing fluid flow.

Core analysis revealed porosity values of about 30% at 140 m depth within heavily altered zones. A similar pattern is observed at the Kivetty site in central Finland, where increased alteration intensity correlates with higher total porosity, improved pore connectivity, and enhanced permeability. Future work will extend hydraulic testing to intervals with high porosity and include fracture aperture and spacing measurements to assess their combined influence. This integrated approach provides a robust framework for distinguishing hydraulically significant fractures from inactive ones, improving site characterization for groundwater resource management, geothermal energy exploration and deep geological repository safety assessments.

How to cite: Okutan, H., Engström, J., Carbajal-Martinez, D., Markovaara-Koivisto, M., Salmi, R., Reijonen, H., and Kortunov, E.: Integrated Characterization of Fracture Orientations and Hydraulic Properties in Crystalline Bedrock, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3278, https://doi.org/10.5194/egusphere-egu26-3278, 2026.

EGU26-3471 | Orals | ERE5.2

Heat transport in deforming fractured rocks: the effects of fracture slip and opening 

Silvia De Simone, Sebastián González-Fuentes, Sandro Andrés, and Víctor Vilarrasa

Heat transfer in fractured rocks is a key process for deep geothermal energy exploitation. Fractures represent the main pathways for fluid flow and advective heat transport, while diffusive thermal exchange occurs between the fluid within the fractures and the surrounding host rock. These two processes occur over very different spatial and temporal scales, and their variability is strongly influenced by fracture–rock heterogeneity, which ultimately controls geothermal performance.

In this work, we discuss two transient mechanical processes that can alter the geometry of fractured rocks during fluid circulation, thereby affecting heat transport and, consequently, the efficiency of geothermal plants. The first process involves flow channeling induced by shear slip activation in critically stressed fractures. We analyze this phenomenon at the single-fracture scale. Using analytical solutions and numerical simulations, we investigate the thermal response to the injection of a cold temperature pulse into a rough fracture, considering both synthetic and real heterogeneous aperture fields. The results reveal that fracture roughness has a significant influence on heat transport, with post-peak tailings of the breakthrough curves showing an anomalous transient decay rate in time before evolving toward the asymptotic regime with a -3/2 decay rate, which is characteristic of fracture-matrix diffusive heat exchange. This behavior is sensitive to variations in the fracture aperture field caused by the activation of relative sliding between fracture surfaces, with larger slips leading to earlier temperature peaks and delayed transitions to the asymptotic diffusive regime.

The second process focuses on cooling-induced thermal contraction of the rock surrounding the fractures, which tends to increase fracture aperture and directly affects fluid flow and advective heat transport. We analyze this phenomenon at the scale of the fractured rock mass. By means of a hybrid methodology that combines an analytical model with a particle tracking approach applied to Discrete Fracture Networks (DFNs), we numerically investigate the impact of cold fluid circulation in systems of fractures with different characteristics. Results show that rock contraction accelerates the advective transport resulting in a faster recovery of cold fluid at the outlet.

These analyses allow identifying the characteristics of fractured rocks that are most critical for heat transport under the occurrence of fracture slip and opening. This understanding is crucial to control the performance and lifetime of geothermal exploitations.

How to cite: De Simone, S., González-Fuentes, S., Andrés, S., and Vilarrasa, V.: Heat transport in deforming fractured rocks: the effects of fracture slip and opening, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3471, https://doi.org/10.5194/egusphere-egu26-3471, 2026.

EGU26-3852 | Orals | ERE5.2

The importance of structural geology in site characterisation of geoenergy and nuclear waste sites  

Jon Engström, Kati Ahlqvist, Sami Vallin, Nikolas Ovaskainen, and Nicklas Nordbäck

Heating and cooling in both industry and households in Europe has become increasingly important but it is still heavily dependent on fossil fuels. Shifting to low-carbon alternatives cuts emissions, strengthens energy security, and enhances the efficiency for these energy systems in the future. These goals can be achieved with a combination of efficient energy storage and clean energy production. Two example solutions within this field are the Cavern Thermal Energy Storage (CTES) and Deep Geological Repositories (DGR), the first used to store thermal energy and the second to solve the waste issue in climate-neutral nuclear energy production. These two solutions have the common requirement of needing advanced structural geological studies. During the last decade research have focused, for example, on developing CTES, which rely on subsurface caverns in low-permeable rocks that are near surface and remain stable when injected with hot and cold water. Today, there is broad international scientific consensus that high-level nuclear waste should not be stored at the surface in the long term. DGR are considered the best solution as they enclose the radioactive waste in suitable host rock formations located several hundreds of meters below the surface. DGR has also been extensively researched and advanced in several countries, and Finland is a global leader in developing the concept for the storage of nuclear waste within crystalline bedrock.

These storage concepts in crystalline bedrock depend on selecting rock blocks that lack major deformation zones and contain few faults and fractures. Hence, the structural geological modelling is an important tool to mitigate uncertainties and to assess the applicability of the bedrock volume for storage. Several methods exist to assess the bedrock, such as non-intrusive geophysical surveys and intrusive drilling of boreholes into the bedrock. State-of-the-art research shows that best results are achieved by combining multiple research methods within a well-designed research framework to define a 3D geological model of the site.   

Successful implementation of these energy storage projects requires the definition of parameters at early stages of the project to define the constrains for the structural geological 3D model. Detailed structural geological modelling enables evaluation of key aspects and mitigation of uncertainties, such as groundwater conditions, seismic risks, mechanical and thermal properties, as well as environmental factors for the project. This exploration approach can significantly reduce time constrains and costs during every step of these projects. In addition, these geological 3D models serve as an important tool for presenting and communicating projects, including their uncertainties, to policy makers, stakeholders and the public.  

How to cite: Engström, J., Ahlqvist, K., Vallin, S., Ovaskainen, N., and Nordbäck, N.: The importance of structural geology in site characterisation of geoenergy and nuclear waste sites , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3852, https://doi.org/10.5194/egusphere-egu26-3852, 2026.

EGU26-4021 | Posters on site | ERE5.2

Capturing natural fracture topology in DFNs for energy and storage applications 

Sarah Weihmann, Christoph Gärtner, James Mullins, Frank Charlier, and Klaus Fischer-Appelt

Many renewable subsurface energy systems rely on understanding fracture networks. In geothermal systems, fractures often provide the primary pathways for fluid flow, while in underground hydrogen storage (UHS) and carbon capture and storage (CCS), fracture networks can strongly influence pressure communication, injectivity or caprock integrity. Similarly, in nuclear waste repositories, fractures can compromise barrier integrity and limit containment. This study investigates the representativity of discrete fracture networks (DFNs) generated from high-resolution photogrammetric outcrop data to support robust models and simulations.

Observed data such as fracture orientations, lengths, intensities, and topological node classifications (X-, Y-, and I-nodes) are used to construct synthetic DFNs via (1) geometric modelling, (2) fracture-growth algorithms, and (3) tracemap extrusion. These DFNs are then meshed and integrated into single-phase flow simulations. Pressure gradients are applied to quantify the influence of fracture intensity and topology on flow behaviour across above fracture generation methods.

Results show systematic topological deviations between natural and synthetic networks. Geometric and growth-based methods overestimate X- and I-nodes while underrepresenting Y-nodes, affecting connectivity and predicted flow paths. Tracemap extrusion reproduces geometry more accurately but requires significantly higher computational resources. Flow simulations reveal that fracture intensity and node topology strongly influence pressure evolution and steady-state attainment. Both parameters are central to injectivity forecasting, (thermal) breakthrough prediction, and storage containment assessment.

Overall, the results demonstrate that current DFN generation methods reproduce fracture geometry reasonably well but struggle to match natural network topology, introducing systematic biases into models and simulations. Improving the representation of Y-node-dominated branching structures is therefore essential for developing more reliable models and simulations of fractured reservoirs and repositories.

How to cite: Weihmann, S., Gärtner, C., Mullins, J., Charlier, F., and Fischer-Appelt, K.: Capturing natural fracture topology in DFNs for energy and storage applications, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4021, https://doi.org/10.5194/egusphere-egu26-4021, 2026.

EGU26-4053 | ECS | Posters on site | ERE5.2

Permeability reduction in fractured geothermal field using heat-activated epoxy resin droplets: resolving droplet transport and adhesion dynamics 

Yutong Cui, Rishi Parashar, Yang Ying, Manish Bishwokarma, and Dani Or

The performance of enhanced geothermal systems (EGS) depends critically on effective water–rock heat exchange. This often requires creation of new fractures, however, for certain scenarios, occluding short-circuiting high flow fractures is needed. Here we introduce an approach for reducing the permeability of large fractures using heat-activated epoxy resin foam. The resin is transported as discrete droplets that become thermally activates (foam, expand and cure) in-situ at a prescribed temperature range. We present modelling and experiments for the transport and adhesion characteristics of resin droplets that result in gradual permeability reduction in large aperture fractures (mm-cm scale). The coupled transport and adhesion of resin droplets is represented in a 2-D numerical model enabling quantification of changes in pressure distribution, flow pathways, and effective permeability. Droplet adhesion considers velocity perturbations coupled with Hertz–Mindlin contact mechanics for thermally activated chemical reaction kinetics. Model predictions show good agreement with laboratory-scale fracture experiments, demonstrating the capability of the proposed approach to capture key mechanisms governing resin sticking and permeability alteration in fractured rock.

How to cite: Cui, Y., Parashar, R., Ying, Y., Bishwokarma, M., and Or, D.: Permeability reduction in fractured geothermal field using heat-activated epoxy resin droplets: resolving droplet transport and adhesion dynamics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4053, https://doi.org/10.5194/egusphere-egu26-4053, 2026.

Faults critically control hydrocarbon migration and accumulation, especially in deep to ultra-deep environments where reservoir quality is generally poor. However, current understanding of fault-controlled hydrocarbon accumulation remains largely qualitative, relying on geological interpretation and conceptual models. A quantitative reconstruction of episodic hydrocarbon expulsion, migration, and accumulation during fault activity under in-situ temperature, pressure, and stress conditions remains lacking, thereby constraining a mechanistic understanding of fault-controlled petroleum systems. In western China, thrust-fault-controlled hydrocarbon reservoirs are widely developed in superimposed basins. This study establishes a geological conceptual model based on typical deep reservoirs, incorporating multiple reservoir–seal assemblages and fault systems. Numerical simulations of hydrocarbon migration and accumulation under fully coupled thermo‑hydro‑mechanical (THM) conditions were conducted using COMSOL Multiphysics. The research quantitatively evaluates the effects of fault geometry, reservoir–seal configurations, and fluid properties on accumulation dynamics. The high-resolution simulations of the fully coupled THM processes reveal that during active faulting periods, hydrocarbons preferentially migrate vertically along the high-permeability damage zone on the fault zone, and are blocked by the seal rock, showing a top-down charging into the reservoirs. During transitional periods, diminished vertical conductivity leads to hydrocarbon accumulation preferentially in proximal, bottom reservoirs. Hydrocarbon enrichment is jointly controlled by fault type (reverse faults being more favorable than normal faults), fault activity sequence, and the relationship between strata and fault tendency. Notably, a “seal-before-break” fault activity pattern can lead to instantaneous release of overpressure-driven hydrocarbons, facilitating highly efficient hydrocarbon accumulation. This study provides a quantitative reconstruction method for fault‑controlled hydrocarbon migration and accumulation under realistic subsurface conditions. It advances the mechanistic understanding of fault‑controlled petroleum systems and offers theoretical support for exploring deep fault‑related reservoirs.

How to cite: Jia, K., Liu, J., and Liu, K.: Hydrocarbon migration and accumulation in a thrust fault-controlled deep reservoir: Insight from the THM coupling numerical modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4203, https://doi.org/10.5194/egusphere-egu26-4203, 2026.

EGU26-4557 | ECS | Orals | ERE5.2

The fault in our clay: Variation in fault cementation in evaporite-bearing mudrocks and implications for sealing 

Griffin Page, Nathaniel Forbes Inskip, Alexis Cartwright-Taylor, Niko Kampman, and Andreas Busch

Mudrocks are a crucial resource for subsurface storage of gases or radioactive waste, both as host rock and caprock. They are characterised by  low primary permeability and high creep rates, limiting the lifespan of fractures, both decreasing the chance of leakage. Large faults pose a significant risk to this, as they act as coupled hydro-mechanical weak points, with potential for increased flow up-dip and along-strike. Gouge generation is well established as a process which limits this permeability increase, however cementation of void space in faults is less well studied.

We studied faults hosted in the Mercia Mudrock Group in the Bristol Channel (southwest UK). We find that gouge and cementation work cyclically with more than one mineral phase, indicating the hydro-mechanical development of a fault through its lifespan. In the fault core, veins tend to be redirected parallel to the mechanical discontinuity between damage zone and gouge, indicating the location of preferential flow. In the damage zone, veins are not always planar in the soft mudrocks and are often part of an anastomosing network which is influenced by other non-fault related structures, such as older veins, sand dyking, and mechanical stratigraphy. The elongated, fibrous gypsum and calcite crystals observed emphasise the importance of high fluid pressures to open and maintain these fractures.

We interpret episodic overpressures that build up layers of gypsum veining in the gouge core of a number of faults; however, the limited special extent of these veins suggests patch-style dilation and slip that may not pose a significant leakage risk. Gypsum veining appears to destroy most remaining evidence of a damage zone in these instances.

This is in contrast to brittle calcite, associated with rifting and inversion, which shows more fluid movement up-and-down-dip and appears to preserve the damage zone. This results in structures that can be reactivated, both by more calcite-bearing fluid but also overpressure caused by rehydration of anhydrite to. This reactivation causes brecciation of the calcite that is not seen in the gypsum despite the overprinting of stress events.

In summary, tectonic environments which open large fault patches potentially pose a higher risk to leakage through mudrock-hosted faults, than fluid overpressure events. However, cementation of these faults, while providing mechanical discontinuities for later dilation events, do appear to seal voids generated by fault activity.

How to cite: Page, G., Forbes Inskip, N., Cartwright-Taylor, A., Kampman, N., and Busch, A.: The fault in our clay: Variation in fault cementation in evaporite-bearing mudrocks and implications for sealing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4557, https://doi.org/10.5194/egusphere-egu26-4557, 2026.

Heating water using waste heat and excess renewable energy in Cavern Thermal Energy Storage (CTES) systems provides a sustainable solution for large-scale thermal energy storage. In addition to challenging economics of CTES, unexpectedly high thermal losses have been a major concern in many cases in the past. In crystalline bedrock, fractured brittle deformation zones can act as fluid pathways, potentially causing thermal losses and compromising cavern stability. Therefore, detailed modelling of these zones is essential for the safe and efficient operation of CTES facilities.

This study presents a workflow for geological characterization and deformation zone modeling at the planned site of the world’s largest CTES facility, VARANTO, in Vantaa, southern Finland. The dataset includes drill core samples totaling over 4 km, acoustic and optical borehole imaging, outcrop observations, and a photogrammetric model. We delineated deformation zone intersections from core samples and classified them into core and damage zones, defining zone dimensions for altered and fractured bedrock. We clustered orientation data from borehole imaging and core logs to determine mean fracture orientations, which, together with zone dimensions, were integrated into a 3D geological model to construct a volumetric representation of deformation zones. Additionally, we parameterized these zones based on properties such as core fracturing, fracture infill, and alteration to characterize and evaluate their structural significance in terms of stability and potential hydraulic conductivity.

The resulting 3D model improves understanding of potential fracture zones and thus pathways for groundwater flow and their impact for thermal and mechanical behaviour, supporting system simulations, monitoring, and maintenance. Representing deformation zones as volumes rather than surfaces enhances integration with groundwater flow models, reduces uncertainty, and enables more accurate prediction of hydraulic connectivity and thermal losses, thereby optimizing system performance. This workflow also provides a transferable methodology for other underground energy storage projects, facilitating risk assessment and design optimization in crystalline bedrock environments.

How to cite: Ahlqvist, K. M., Engström, J., Vallin, S., and Hagström, M.: Geological 3D modeling in crystalline bedrock for a cavern thermal energy storage site in S Finland - defining properties and parameters for deformation zones, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4833, https://doi.org/10.5194/egusphere-egu26-4833, 2026.

EGU26-4886 | ECS | Posters on site | ERE5.2

Preparation of fracture data and delineation of bedrock domains for 3D DFN modeling of a cavern thermal energy storage site in Southern Finland 

Teemu Lindqvist, Kati Ahlqvist, Jon Engström, and Markku Hagström

Cavern thermal energy storage (CTES) is increasingly recognized as a key technology for integrating renewable energy sources and balancing seasonal heat supply and demand. The implementation of CTES in crystalline bedrock settings requires detailed characterization of brittle deformation zones and fracture networks that both control heat transfer and cavern stability. Site-scale zones of localized brittle deformation, ranging from tens of centimetres to several metres in thickness and tens to hundreds of metres in length, can often be identified from drillcore interpretations and represented deterministically in structural geological models. In contrast, fracture networks are commonly constrained by sparse observations of individual fractures with small apertures, necessitating stochastic approaches to account for limited sampling and uncertainty within poorly constrained subsurface volumes. Consequently, detailed fracture mapping and classification, together with the identification of volumes of bedrock constrained by the deformation zones, i.e. bedrock domains, are essential prerequisites for fracture network modelling that utilize, for example, Discrete Fracture Network (DFN) approaches.


In this study, we evaluate the usability of the conventionally acquired and subsequently classified fracture data for generating fracture sets for 3D DFN models in crystalline bedrock deformed by multiple tectonic events and comprising variably altered granites and gneisses. We also evaluate brittle deformation zones as constraints for determining structurally homogeneous bedrock domains. The study focuses on the planned largest CTES site in the world, VARANTO, located in Vantaa, southern Finland, with an approximate storage volume of 1 million m³ and a heat capacity of 90 GWh. The dataset comprises optical or acoustic borehole images (OBI and ABI) from 36 boreholes, fracture observations from oriented drillcores and field observations, and 3D deformation zone models available from earlier work.


The results indicate that classification of discontinuities from the OBI and ABI images based on filling type can present challenges in distinguishing between brittle fractures and other structures such as dikes without a brittle interface. In addition, variations in the OBI and ABI image quality may lead to intervals with limited or less distinct observations. These findings highlight the value of integrating supplemental data sources, such as the fractures mapped from oriented drill cores and field observations, to enhance interpretation and overall representativity of the fracture data. Moreover, using the deformation zone models to constrain the bedrock domains results in a domain pattern that is challenging in terms of drillhole fracture data availability for DFN modeling. Therefore, we briefly discuss filtering of the domains based on available data.

How to cite: Lindqvist, T., Ahlqvist, K., Engström, J., and Hagström, M.: Preparation of fracture data and delineation of bedrock domains for 3D DFN modeling of a cavern thermal energy storage site in Southern Finland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4886, https://doi.org/10.5194/egusphere-egu26-4886, 2026.

EGU26-6253 | Orals | ERE5.2

Why late-stage collisional orogens are favorable for geothermal exploration 

Marco Herwegh, Timothy Schmid, Daniela B. van den Heuvel, Christoph Wanner, Larryn W. Diamond, James Faulds, Alfons Berger, Tobias Diehl, and Herfried Madritsch

In contrast to convergent plate tectonics during subduction, collisional orogens in their late stages (e.g., Alps, Pyrenees, Himalayas) typically exhibit little to no magmatic activity. Consequently, these settings have historically received limited attention in exploration for geothermal energy. Nevertheless, such orogens do host active, amagmatic geothermal systems owing to the co-occurrence of several key features: (1) ongoing crustal-scale deformation within the brittle upper crust, which generates spatially dispersed, permeable fracture networks; (2) major, steep strike-slip and normal faults with permeable dilation zones that cut across the fracture networks; (3) geothermal gradients of 20–35 °C/km, which provide heat to circulating fluids; (4) pronounced topographic relief, which induces strong hydraulic head gradients between high surface elevations and valley floors.

The interaction of these features produces dynamic geothermal circulation systems: meteoric water infiltrates at high elevations into the dispersed fracture networks and is focused into the major faults, allowing the water to descend to depths up to 10 km and become heated to above 200 °C. Subvertical dilation zones within the major faults link the deep flow paths to the surface or relatively shallow depths, generally at lower elevations, allowing the topographically induced hydraulic gradients to drive the hot water up to discharge sites in the valley floors.

Unfortunately, in orogens where valleys are glacially over-deepened, outflow is commonly hidden under thick sequences of unconsolidated sediments. Therefore, the challenge in exploration in such settings is to locate these blind geothermal systems. To address this challenge, we examined the geothermal favorability of the mountainous Valais region in SW Switzerland, which is one of the most well-known areas of geothermal activity in the European Alps. Through collaboration among structural geologists, hydrogeochemists and seismologists, all available geological and hydrochemical data were compiled in a GIS database to conduct a Play Fairway Analysis. Each data layer was evaluated and rated for its ability to directly or indirectly indicate sites of deep thermal upflow. By weighting and combining these layers, we produced favorability maps displaying areas where active upflow of thermal water is most likely. A notable outcome is that most of the known thermal springs in the study area fall within the identified favorable areas. This success demonstrates the usefulness of the favorability maps in guiding more spatially-targeted exploration in the Valais region. Moreover, our methodology provides a transferable framework for exploration in similar geodynamic settings elsewhere.

How to cite: Herwegh, M., Schmid, T., van den Heuvel, D. B., Wanner, C., Diamond, L. W., Faulds, J., Berger, A., Diehl, T., and Madritsch, H.: Why late-stage collisional orogens are favorable for geothermal exploration, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6253, https://doi.org/10.5194/egusphere-egu26-6253, 2026.

EGU26-7692 | Orals | ERE5.2

A massive hydraulic tomography experiment for the high-resolution characterization of the excavation induced fracture network using a travel-time based inversion scheme 

Ralf Brauchler, Axayacatl Maqueda, Rémi de La Vaissière, Médéric Piedevache, and Alain Laurent

The Meuse/Haute-Marne Underground Research Laboratory hosts a large-scale hydraulic tomography experiment designed to characterize fracture networks induced around open and sealed galleries. The objective of this study is to reconstruct their hydraulic properties and fracture geometry to validate a conceptual model describing stress redistribution during tunnel excavation. In the first step, cross-hole responses from gas permeability tests conducted by Solexperts SA were analyzed using an equivalent porous media approach consisting of a 3D travel-time-based tomographic inversion. In the second step, a sequential inversion scheme was applied to reconstruct discrete fracture planes in 3D.

Gas injection tests were carried out across 11 boreholes, each equipped with a movable multi-packer system comprising six intervals for injection or observation. This configuration enabled the recording of 1168 pressure interference signals with a signal-to-noise ratio sufficient for inversion.

The applied 3D travel-time-based tomographic approach relies on transforming the transient groundwater flow equation into the eikonal equation using an asymptotic approximation. This inversion method allowed reconstruction of the 3D gas diffusivity distribution, capturing the key features of the conceptual model related to stress redistribution during excavation. The sequential inversion approach integrates the 3D travel-time inversion with multivariate statistics and basic geological constraints. This method enables significant mesh refinement within the model domain while avoiding a strong ill-posed inversion problem. It successfully reconstructed fracture traces of the induced network parallel to the tunnel surface, including both extension and shear fractures.

Combining results from both approaches enhanced understanding of the spatial geometry of the induced fracture network around galleries: the 3D travel-time tomography provided a comprehensive spatial representation of the conceptual model, while the sequential inversion delivered high-resolution 3D images of fracture traces associated with its main properties.

How to cite: Brauchler, R., Maqueda, A., de La Vaissière, R., Piedevache, M., and Laurent, A.: A massive hydraulic tomography experiment for the high-resolution characterization of the excavation induced fracture network using a travel-time based inversion scheme, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7692, https://doi.org/10.5194/egusphere-egu26-7692, 2026.

EGU26-8504 | Orals | ERE5.2

Development of Large-scale Rock Friction Apparatuses at NIED, Japan 

Eiichi Fukuyama, Futoshi Yamashita, Shiqing Xu, Kazuo Mizoguchi, Hironori Kawakata, Kurama Okubo, Yoshiyuki Matsumoto, and Sumire Maeda

Development of large-scale rock friction apparatus started around 2010 at National Research Institute for Earth Science and Disaster Resilience (NIED) in Japan (Fukuyama et al., 2014, NIED Rep.). Until now, three generations of the apparatus have already been developed, whose sliding area ranges from 1.5 m to 6.0 m in length. The purpose of this project was to investigate the rock frictional properties and earthquake rupture process at various sliding scales. There are two important characteristics in these apparatuses. One is that the nucleation zone size can be generated within the sliding fault area. The other is that the nucleation process can be spatially monitored by local strain measurement array installed close to the sliding surfaces. When nucleation zone is confined to the experimental fault surfaces, the whole rupture process from initiation to termination could be able to be observed in the experiments (Yamashita et al., 2026, EGU). Using these apparatuses, many kinds of large-scale rock friction experiments have been conducted. Through such experimental research, the following results have been reported. 1) The spatial distribution of strength on the fault surface is heterogeneous, which had not been properly considered by small-scale experiments (Yamashita et al., 2015, Nature). 2) Such spatial heterogeneity of strength on the fault surface could contribute to the fault-size dependence of macroscopic rock friction as well as the rich spectrum of rupture behaviors, which are quite important for the modeling of earthquake generation process (Xu et al., 2023, Nat. Geosci.). Especially, due to high-speed loading (~1 mm/s) and long-distance sliding (~40 cm), ten-decimeter-scale heterogeneity on the fault surface could be generated, which is found to play an important role in large-scale friction experiments (Yamashita et al., 2018, Tectonophys.). In addition to these spatially heterogeneous fault friction experiments, rupture propagation has been investigated in detail to investigate the fracture energy (Okubo et al., 2026, EGU; Matsumoto et al., 2026, EGU). In the near future, we expect that such large-scale rock friction experiments would contribute significantly to seismology, especially, physics of earthquake generation process, by establishing new constitutive law(s) of the rock friction through the usage of dense arrays of near-fault observations.

How to cite: Fukuyama, E., Yamashita, F., Xu, S., Mizoguchi, K., Kawakata, H., Okubo, K., Matsumoto, Y., and Maeda, S.: Development of Large-scale Rock Friction Apparatuses at NIED, Japan, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8504, https://doi.org/10.5194/egusphere-egu26-8504, 2026.

Abstract: Early-term inactive faults can be reopened as hydrocarbon migration channels under overpressure. Clarifying their opening mechanism during the hydrocarbon accumulation period is the foundation of hydrocarbon exploration. In view of the problem that early-term inactive faults in the Junggar Basin have the potential for cross-layer migration but the overpressure-driven opening mechanism is unclear, this study constructs a mechanical model coupled with strong and weak layer combinations and pore fluid pressure. Combined with the Mohr-Coulomb fracture criterion, the mechanical response characteristics of the faults under two boundary conditions of lateral confinement and unconfined confinement are analyzed, thereby revealing the opening mechanism of early-term inactive faults. The study shows that: (1) Under lateral confinement conditions, the overpressure evolution is in two stages: "Mohr circle translation - radius enlargement". Due to stress distribution, the Mohr circle is preferentially tangent to the original fracture line, which promotes the local opening of the fault. (2) Under lateral unconfined confinement conditions, the effective stress change is concentrated on the fracture surface, driving the Mohr circle to the left and reducing the critical stress value for opening early-term inactive faults. (3) Both laterally restricted and laterally unrestricted states exhibit the characteristics of "priority of overpressure zone, dominance of lower fault, and initial opening of overpressure segment", and can further extend along the original fault. (4) The study area as a whole shows that the critical opening pressure of the western fault is higher than that of the eastern fault, and this pressure has shown an evolution trend of "increasing-decreasing-increasing" since the end of the Triassic. Areas closer to the overpressure center of the source rock and with a smaller angle between the fault strike and the maximum principal stress have better opening properties. In the late hydrocarbon accumulation stage, some early-decaying faults open due to the overpressure reaching the critical condition, and can serve as effective hydrocarbon migration channels.

How to cite: Zhang, W. and Liu, H.: Research on the Opening Mechanism of Early-Term Inactive Faults: A Case Study of the Junggar Basin, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9318, https://doi.org/10.5194/egusphere-egu26-9318, 2026.

EGU26-9512 | ECS | Orals | ERE5.2

Electric Self-Potential Measurements during Fluid Injection at the Bedretto Underground Laboratory 

Nadine Haaf, Jeroma Azzola, Liliana Vargas Meleza, Marian Hertrich, Valentin Gischig, Mathilde Wimez, Antonio Pio Rinaldi, Fridolin Straub, Maren Brehme, Domenico Giardini, Francisco Sorbeto, and Andreas Alcolea

Self-potential (SP) monitoring was implemented at the Bedretto Underground Laboratory as part of the BEACH experiment to complement multi-parameter observations during fluid-injection tests. Continuous SP measurements have been conducted since the end of October 2025, with data acquired so far covering the period until mid-December, and monitoring planned to continue throughout the current year.

The SP setup consists of nine non-polarizable Pb/PbCl₂ electrodes installed along the tunnel wall and within one borehole in the Mesozoic Crystalline Fault Zone. Tunnel-wall electrodes were placed in shallow drill holes and embedded using conductive contact material to ensure stable long-term coupling to the rock. A single electrode was installed in a 50m borehole to provide additional depth sensitivity. All electrodes were connected to a CR6 data logger, recording continuous SP time series with a sampling interval of one value per minute.

The recorded data span different operational phases, including background conditions as well as cold and warm water injection cycles and associated shut-in periods. This contribution presents an initial overview of the acquired SP dataset.

 

 

 

Acknowledgements:

BEACH – Energie Speicherung und Zirkulation von Geothermischer Energie in Bedretto receives funding from the Swiss Federal Office of Energy (SFOE), Project number SI/502817.

"Geo-INQUIRE is funded by the European Commission under project number 101058518 within the HORIZON-INFRA-2021-SERV-01 call."

How to cite: Haaf, N., Azzola, J., Vargas Meleza, L., Hertrich, M., Gischig, V., Wimez, M., Rinaldi, A. P., Straub, F., Brehme, M., Giardini, D., Sorbeto, F., and Alcolea, A.: Electric Self-Potential Measurements during Fluid Injection at the Bedretto Underground Laboratory, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9512, https://doi.org/10.5194/egusphere-egu26-9512, 2026.

EGU26-10407 | ECS | Posters on site | ERE5.2

Structural Characteristics and Genesic Mechanism of Antiformal Negative Flower Structures: Insights from the Doseo Basin, Central-West African Rift System 

Yu Yang, Yifan Song, Kunye Xiao, Yebo Du, Xinshun Zhang, Li Wang, Yafei Ou, and Ying Hu

Unlike classical positive and negative flower structures, antiformal negative flower structures represent a unique structural type developed under strike-slip tectonic inversion regimes. Rarely reported in previous studies, the genesic mechanism of such structures remains poorly understood, particularly the mechanical reasons that inhibit the inversion of pre-existing normal faults under compressional conditions. Based on detailed interpretation of high-resolution seismic data, this study systematically investigates the tectonic setting, structural characteristics, and formation mechanism of antiformal negative flower structures in the Doseo Basin of the Central–West African Rift System, and discusses their implications for the structural evolution of strike-slip inversion basins and the development of hydrocarbon traps.

The Doseo Basin is located within the basin-controlling domain of the Central-West African Rift System and experienced two major tectonic episodes: transtension during the Early Cretaceous and intense tectonic inversion during the Eocene. These tectonic events resulted in the development of multiple types of inversion-related structures, including fault-associated, thrust-related, fold-dominated, and antiformal negative flower structures. Antiformal negative flower structures are mainly developed within the central low-relief uplift belt of the basin. In planar view, these structures are arranged in en echelon with a NWW-SEE trend, whereas in cross-section they are characterized by an antiformal uplift controlled by a set of normal faults. During the inversion stage, the pre-existing normal faults were not reactivated to reverse faults; instead, the strata experienced pronounced compressional arching. Notably, the spatial extent of the anticlinal uplift closely coincides with the distribution of the normal faults. Genetic analysis indicates that under the Early Cretaceous transtensional stress field, basement weak zones were reactivated, leading to the formation of normal faults and the initial development of negative flower structures. During this stage, the scale, vertical extent, and activity intensity of the normal faults were established. During the Eocene tectonic inversion, regional transpressional stress was superimposed on the negative flower structure system. However, constrained by two key factors, the relatively high mechanical stability of the early transtensional structures (related to fault cementation and lithological properties of surrounding rocks) and high dipping of the normal faults, the inversion-stage stress failed to reach the critical threshold required for fault polarity reversal. Instead, it was only sufficient to induce compressional arching of the strata, ultimately resulting in antiformal negative flower structures characterized by the preservation of pre-existing normal faults combined with an antiformal uplift.

This study demonstrates that the preservation of normal faults is jointly controlled by insufficient inversion-stage stress and the mechanical stability of pre-existing transtensional fault systems. These findings expand current genetic models of structural styles in strike-slip inversion basins and provide new geological constraints for structural interpretation and hydrocarbon trap prediction in the Doseo Basin and other analogous basins.

How to cite: Yang, Y., Song, Y., Xiao, K., Du, Y., Zhang, X., Wang, L., Ou, Y., and Hu, Y.: Structural Characteristics and Genesic Mechanism of Antiformal Negative Flower Structures: Insights from the Doseo Basin, Central-West African Rift System, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10407, https://doi.org/10.5194/egusphere-egu26-10407, 2026.

EGU26-11471 | ECS | Orals | ERE5.2

Fracture network modeling with graph deep learning 

Ana Paula Burgoa Tanaka, Philippe Renard, Xiao Xia Liang, Julien Straubhaar, and Dany Lauzon

Most existing fracture modeling workflows rely on the generation of discrete fracture networks (DFN), which simulate fracture patches based on stochastic distributions of geometric parameters and generally neglect topological constraints. To address the DFN constraints, we propose applying graph theory and deep learning to characterize and generate coherent fracture networks from real-world datasets. Our approach broadens the range of quantitative methods available for fracture modeling; it is non-gridded and accounts for both geometry and topology in the generation of new networks. 

The generation of fracture networks based on a reference and/or analog network interpretation is useful for modeling subsurface uncertainties related to fracture positions and network intersections. This application is useful for sites where fracture interpretation is possible, but where full coverage of the study site is not available. For characterization, we integrate geometry, topology, kinematics, age relationships, and geomechanics to identify the most important connections within a network. For simulations, we combine a graph recurrent neural network (GraphRNN) for generating graph topology and graph denoising diffusion probabilistic models (DDPM) for generating node positions in space. Deep generative models learn distributions from the training fracture network data and generate new networks with a variable number of fracture lineaments, represented as edges, while intersections are represented as nodes.

Our method is applied to a real case study from the Western Helvetic Alps domain in Switzerland. The model is trained on graphs derived from the fracture network interpretation of a Cretaceous limestone aquifer. The generation of new fracture networks as graphs yields coherent topologies with statistical distributions similar to those of the training data for node degree and relative node positions (i.e., edge length and azimuth). Furthermore, the training dataset and the generated networks are compared using node centrality measures (betweenness and percolation), which help describe the network's connectivity and highlight preferential flow paths, thereby emphasizing the role of fracture connectivity in enhancing permeability and controlling flow anisotropy. The method is promising for the generation of fracture networks as an alternative approach that can be used to identify preferential fluid flow paths and to build scenarios for later flow simulation for hydrogeology, reservoir management, geothermal energy, nuclear waste disposal, and geologic sequestration.

How to cite: Burgoa Tanaka, A. P., Renard, P., Liang, X. X., Straubhaar, J., and Lauzon, D.: Fracture network modeling with graph deep learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11471, https://doi.org/10.5194/egusphere-egu26-11471, 2026.

EGU26-11476 | ECS | Orals | ERE5.2

Hydro-mechanical loading effects on flow through a single natural fracture 

Brandon Stock, Andrew Frampton, and Diego Mas Ivars

Fractured crystalline rocks are widely regarded as suitable host formations for waste isolation applications, including deep geological repositories for spent nuclear fuel. Fluid flow in these systems is predominantly controlled by networks of fractures whose hydraulic properties are governed by internal heterogeneity, contact area distribution, and stress-dependent aperture evolution. These properties are strongly influenced by in situ stress conditions, which may evolve over geological to engineering time scales due to processes such as glacial loading, stress redistribution, and excavation-induced damage. Robust representation of fracture-scale flow behaviour is therefore critical for the development and calibration of large-scale discrete fracture network models.

In this study, we investigate the coupled hydro-mechanical behaviour of a natural single fracture using a laboratory-scale flow experiment under increasing normal load. The fracture aperture field was reconstructed using high-resolution 3D scanning of the opposing fracture surfaces, with vertical alignment refined using pressure-sensitive film measurements. A systematic sensitivity analysis of 27 alignment cases, incorporating translational uncertainties along the x-, y- and z-directions was performed to quantify their influence on flow behaviour. Measured flow rates were compared against predictions from the local cubic law under varying normal stress. Results demonstrate that flow is highly sensitive to fracture surface alignment, with misalignment along the flow direction and normal direction exerting the dominant influence. The local cubic law systematically overestimates flow by at least two orders of magnitude for all loading cases. Furthermore, the application of a constant correction factor to convert mechanical to hydraulic aperture, calibrated under unloaded conditions, fails to reproduce experimental flow rates as normal load increases. We propose a stress-dependent correction factor linked explicitly to the evolution of fracture contact area. Incorporating this relationship yields close agreement with experimental observations across all loading and alignment cases.

How to cite: Stock, B., Frampton, A., and Mas Ivars, D.: Hydro-mechanical loading effects on flow through a single natural fracture, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11476, https://doi.org/10.5194/egusphere-egu26-11476, 2026.

Ensuring the safe disposal of high-level radioactive waste in a suitable host rock requires compliance with several legally defined criteria. In Germany, these criteria are established by Repository Site Selection Act (Standortauswahlgesetz – StandAG). One of the key hydrogeological criteria constrains the hydraulic conductivity of the host rock to values below 10-10 m/s. In crystalline rocks, hydraulic conductivity is governed by contributions from both the rock matrix and the fracture network, with transport typically dominated by fractures.

Fractures are characterized by multiple parameters, including orientation (strike and dip angles), fracture size (strike and dip lengths), volumetric fracture density (number of fractures per unit volume), and hydraulic aperture. The main objectives of this study are to (i) evaluate the sensitivity of effective hydraulic conductivity to individual fracture parameters and their correlations, (ii) test a DFN-based workflow for hydraulic upscaling at the representative elementary volume (REV) scale, and (iii) identify parameter combinations that satisfy the hydraulic safety criterion defined by StandAG for nuclear waste repositories.

Parameter correlations represent dependent relationships between fracture properties. Semi-correlated DFN models account for relationships between fracture aperture, strike length, and fracture density while incorporating a stochastic term to capture natural variability, whereas uncorrelated DFN models assume full parameter independence.

Both semi-correlated and uncorrelated DFN models were considered to investigate the influence of correlations between fracture length, aperture, and volumetric fracture density on hydraulic behavior. The proposed workflow integrates DFN generation using the software Frackit, the upscale of fracture-scale properties to an equivalent porous medium (EPM) based on Oda’s method assuming cubic-law fracture-scale flow, and flow simulations performed with FEFLOW 10 to derive effective hydraulic conductivity.

The DFNs were generated within a cubic volume of 50×50×50 m³. Fracture lengths range from a few to several tens of meters, volumetric fracture densities vary between approximately 10-4 and 10-2 m-3, strike and dip angles span 0–180° and 0–90°, respectively, and fracture apertures extend from 10-7 to 10-2 m.

The results show that (1) fracture aperture was consistently found to be the strongest parameter controlling hydraulic conductivity in both semi-correlated and uncorrelated models. In semi-correlated models, volumetric fracture density and fracture dimensions such as strike and dip lengths also significantly affect the effective hydraulic conductivity. Strike and dip angles exhibited low sensitivity. In uncorrelated models, the aperture alone dominates flow, while other parameters show negligible influence. (2) Effective hydraulic conductivity compatible with the StandAG limit is typically found when fracture apertures are small, i.e., smaller than 10-4 m, strike lengths are short, i.e., shorter than 10 m, and fracture density is moderate to high, i.e., higher than 1 × 10-3 m-3, in semi-correlated models. In uncorrelated models, hydraulic conductivity below the standard limit is primarily controlled by small apertures, i.e., smaller than 10-4 m, independent of fracture density.

How to cite: Jimenez, V. and Renz, A.: Sensitivity analysis of fracture parameters in discrete fracture network (DFN) models for effective hydraulic conductivity under StandAG, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12023, https://doi.org/10.5194/egusphere-egu26-12023, 2026.

EGU26-13002 | ECS | Orals | ERE5.2

Transient permeability in ductile rocks: the competition between deformation and healing 

Gabriel Meyer, Francesco Lazari, and Marie Violay

Fluid circulation in ductile rocks controls the deposition of critical resources such as copper and molybdenum, as well as the potential for deep, supercritical geothermal systems. However, the mechanisms that allow or hinder such circulation under high temperature and pressure conditions remain poorly understood.

In this study, we conducted two sets of healing experiments on thermally cracked Lanhelin granite, both water-saturated and dry, under high confining pressure and temperature. The first set of experiments was carried out under hydrostatic conditions (Peff = 85 MPa) with increasing temperature (21–400 °C). The second set was conducted under triaxial conditions, in which specimens were deformed at Peff = 85 MPa, temperatures ranging from 200 to 600 °C, and a strain rate of 10⁻⁶ s⁻¹. In both cases, permeability was continuously recorded throughout.

Under hydrostatic conditions, permeability remained roughly constant at room temperature and in dry samples, but decreased by up to an order of magnitude over 8 hours at 400 °C. Under triaxial deformation, water-saturated specimens were weaker and exhibited more ductile behavior compared to dry samples. Moreover, the more ductile the sample, the greater the increase in permeability observed leading up to failure.

Microstructural evidence supports chemical crack self-healing as the dominant healing mechanism in the hydrostatic experiments. In the deformed samples, post-mortem analysis revealed that the observed increase in permeability is associated with pervasive cracking throughout the bulk of the rock.

Overall, our study demonstrates the necessity of deformation to generate permeability in ductile rocks, while also highlighting the transient nature of this permeability.

How to cite: Meyer, G., Lazari, F., and Violay, M.: Transient permeability in ductile rocks: the competition between deformation and healing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13002, https://doi.org/10.5194/egusphere-egu26-13002, 2026.

EGU26-13705 | ECS | Orals | ERE5.2

Fault-controlled paleofluid flow in shale caprocks: Structural, geochemical, and mineralogical evidence from the Bristol Channel Basin (UK) 

Tunahan Aykut, Nicolas Beaudoin, Christopher Wibberley, Jade Dutilleul, Laurent Emmanuel, and Jean-Paul Callot

Understanding the development of fault zones in caprock shales and their impact on permeability is critical when considering underground CO2 storage in aquifers and depleted reservoirs. To enhance this knowledge, we characterize the paleofluid system in seismic-scale faults cutting through low-permeability shale formations, assesing whether fluids recorded in the fault core and damage zone record large-scale migration and enhanced effective permeability. The Somerset coast (UK), along the southern margin of the Bristol Channel Basin, exposes shale and marl dominated Mesozoic caprock successions dissected by seismic-scale normal and inverted faults, of which the timing of initial activity is well constrained by radiochronology and which exhibit well-preserved fault cores and damage zones as well. In this study, we present field-based structural analyses, petrographic investigations, stable isotope geochemistry (δ¹³C, δ¹⁸O) and clay mineralogy (XRD) from six selected outcrops. The vein-rich damage zones exhibit calcite and gypsum precipitation, recording transient fluid-flow episodes during reactivation. Stable isotope data, combined with fluid inclusion petrography, indicate that these episodes were dominated by meteoric fluids (δ¹⁸O<-10‰ VPDB) from which synkinematic calcite precipitated in faults at geothermal conditions (<60°C). When considering published radiogenic ages for the extensional development (150-120 Ma) and subsequent inversion (50-20 Ma) of the considered faults, the recharge of meteoric fluids in the fault at depth is consistent with regional paleogeographic reconstructions showing fluctuating emergence of landmasses in the area during the Late Triassic to Cretaceous. Within this framework of episodic fluid circulation, most fault cores are mechanically sealed rather than swelling-sealed, with permeability reduction controlled by grain-size reduction and the development of aligned clay fabric. Nevertheless, mineralized fault cores demonstrate that fault sealing is not static, during episodes of elevated fluid pressure or reactivation, permeability may be locally and temporarily enhanced along discrete slip surfaces. This behavior is strongly controlled by fault-zone architecture, with increasing displacement promoting gouge thickening and fabric development, ultimately leading to more effective long-term sealing. Beyond regional implications, our study reconstructs kilometer-scale downward fluid-flow along faults, supporting the significant impact of the damage zone on the long-term integrity of clay-rich caprocks.

How to cite: Aykut, T., Beaudoin, N., Wibberley, C., Dutilleul, J., Emmanuel, L., and Callot, J.-P.: Fault-controlled paleofluid flow in shale caprocks: Structural, geochemical, and mineralogical evidence from the Bristol Channel Basin (UK), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13705, https://doi.org/10.5194/egusphere-egu26-13705, 2026.

EGU26-14875 | Posters on site | ERE5.2

Hydraulic fracturing of the transverse isotropic argillite from Tournemire in a hollow cylinder triaxial cell: experimental study and analytical modelling 

Dragan Grgic, Albert Giraud, Coffi Gbewade, Bastien Walter, and Mohamed Moumni

To study the effect of hydraulically induced damage in a caprock (argillite from Tournemire), hydraulic fracturing tests were conducted in a hollow cylinder triaxial cell on core samples with inner borehole, oriented parallel to the bedding plans. Acoustic Emission (AE) monitoring and strain measurements during hydraulic fracturing tests, as well as post-mortem X-ray CT analysis were carried out. Samples were subjected to stresses representative of the in-situ stress state, and different injection rates of low-viscosity fluid (water) were tested.

Overall, the breakdown pressure is higher and AE activity due to microcracking damage (which increases almost simultaneously with the pressure drop) appears earlier when the injection flow rate increases. During the second injection phase, peak pressures are lower, pressurization rates are higher and stress-strain behaviour is stiffer. The analysis of values of Rise Angle (RA) and Average Frequency (A-FR) indicates that increasing the injection flow rate generates more tensile cracks and increases the severity of damage. The cumulative damage variable, calculated from AE activity, increases significantly just before the first pressure drop and this increase is stiffer when the injection flow rate increases. This confirms that the use of a low-viscosity fluid (water) induces the propagation of unstable cracks, which initiate almost simultaneously with the pressure drop in the borehole, and that this propagation is faster for higher injection rates.

The breakdown pressure and the crack orientation are analysed thanks to the elastic theory for transverse isotropic materials and chemo-hydro-mechanical coupled processes at the borehole wall. The analysis of core samples deformations and X-ray images, and post-mortem visual observation of samples surface indicate that cracks are primarily oriented parallel to the bedding planes and the core sample axis.

How to cite: Grgic, D., Giraud, A., Gbewade, C., Walter, B., and Moumni, M.: Hydraulic fracturing of the transverse isotropic argillite from Tournemire in a hollow cylinder triaxial cell: experimental study and analytical modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14875, https://doi.org/10.5194/egusphere-egu26-14875, 2026.

Fluid injection into fractured crystalline rock enhances permeability by opening new fractures and reactivating natural ones, yet the relative roles of fluid pressure and elastic stress transfer remain insufficiently constrained. In this study, we develop a fully coupled hydro-mechanical Particle Flow Code in 3 Dimensions (PFC3D) model calibrated against two mini-frac tests in Rotondo Granite at the Bedretto Underground Laboratory. Applied to intact and naturally fractured intervals, the model reproduces the observed pressure evolution and enables quantitative analysis of fracture slip and stress redistribution, thereby revealing two distinct reactivation mechanisms. The first mechanism arises from effective stress reduction. Elevated pore pressure lowers the effective normal stress and weakens frictional resistance, leading to localized and directionally consistent shear within the high-pressure core. Weaker and more diffuse slip develops outward following the pattern of elastic stress perturbation, and minor shear failure appears at the far edge of the fluid-affected region due to shear stress transfer acting on the compressed faces of the opening fracture. This spatially hierarchical slip structure reflects a transition from deformation dominated by effective stress reduction to deformation dominated by elastic stress transfer. The second mechanism is governed by elastic stress transfer. Deformation of pressurized fractures redistributes surrounding stresses and induces weak, remote shear on neighboring fractures that remain disconnected from the fluid. The resulting stress perturbation resembles that generated by localized volumetric expansion and promotes slip on nearby fractures. An analytical estimate indicates that the radial extent of stress perturbation exceeds the fluid-pressurized region and increases with injected volume while decreasing with rock stiffness. These results establish a unified, field-calibrated framework linking fluid pressure, fracture deformation, and stress redistribution during hydraulic stimulation.

How to cite: Shen, H., Hofmann, H., Zang, A., Zhang, S., Zhou, J., and Yoon, J. S.: Reactivation of Natural Fractures Driven by Fluid Pressure and Stress Transfer During Hydraulic Stimulation: A Three-Dimensional Discrete Element Modeling Study of the Bedretto Underground Laboratory, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14876, https://doi.org/10.5194/egusphere-egu26-14876, 2026.

Fractures significantly control subsurface heat and fluid transport and the mechanical properties of rock formations. Natural and stimulated fracture growth processes are thus essential for production of oil and gas in conventional and unconventional reservoirs, caprock integrity, underground storage of carbon dioxide, hydrogen, or wastewater, and for geothermal energy production in systems that require fracture stimulation or that depend on natural fractures for heat extraction. While the formation of fractures is conventionally seen as a purely mechanical process, chemical processes can decrease or increase the propensity for fracture growth as a function of stress conditions, fluid chemical and physical environment, rock composition, and rate of change of fracture driving loading conditions. The influence of chemical reactions on rock fracture processes and their implications for subsurface energy resources is thus increasingly recognized.

In combination with field structural observations of fractures in a variety of natural settings, we conduct double torsion fracture mechanics tests for sandstone, shale, and polycrystalline halite to quantify effects of fluid chemical environment on fracture mechanical properties. Tests are conducted under a range of fluid compositional and environmental conditions that are relevant to subsurface hydrogen and CO2 storage and geothermal energy production. Double torsion fracture mechanics tests measure fracture toughness and subcritical fracture index. Fracture toughness quantifies the loading stress for critical fracture growth, and subcritical fracture index the rate of fracture propagation under subcritical loading conditions. Tests are conducted under ambient room conditions, in dry N2, CO2, or H2 gas environments, and partially or completely saturated aqueous conditions. Some materials are also reacted in an autoclave under elevated temperature and pressure conditions in the presence of H2 and N2 gas prior to fracture testing.

Both fracture toughness and subcritical fracture index are influenced by the chemical environment to varying degree dependent on rock mineral composition, fluid composition, and environmental conditions. For all rock types except polycrystalline halite, samples tested under dry conditions have higher toughness and subcritical index values compared to partially or fully water-saturated samples. This can be beneficial for caprock integrity of CO2 or H2 storage reservoirs where injected gas would dry out the formation reducing the tendency for fracture-controlled leakage of top seals. Aqueous chemical reactions triggered by H2 or CO2 gas injection in porous reservoirs can both impede and enhance mechanical fracture processes depending on the combined effects of mineral dissolution and concurrent precipitation of newly formed minerals. With increasing temperature, the effects of aqueous mineral reactions on fracture properties are generally more pronounced, demonstrating the significance of reactive fracture processes in conventional and enhanced geothermal reservoirs. It is envisioned that chemical effects of fracture growth can be utilized to reduce undesired fracture growth or to optimize stimulated fracture growth to obtain desired fracture geometries that benefit subsurface energy operations.

How to cite: Eichhubl, P. and Gajda, D.: Fracture growth under reactive subsurface conditions: Processes, Mechanisms, and Significance for Geoenergy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15090, https://doi.org/10.5194/egusphere-egu26-15090, 2026.

EGU26-18678 | ECS | Orals | ERE5.2

A Comparative Study of Deterministic and Stochastic DFN Models for Rock Mass Hydraulic Property Estimation 

Marina Facci, Silvia Favaro, Stefano Casiraghi, Federico Agliardi, Silvia Mittempergher, Waqas Hussain, Jeffrey Hyman, Ramil Gainov, Oleksandr Slipeniuk, Massimo Fogazzi, and Andrea Bistacchi

Discrete Fracture Network (DFN) models are widely used for predicting the hydraulic properties of heterogeneous fractured rock masses through the implementation of diverse numerical and semi-analytical methods. However, recent advancements in the parametrization of fracture networks by statistical analyses of field and geophysical data are not yet fully integrated into the capabilities of standard DFN simulators. Available 3D stochastic DFN generators (i) lack the ability to produce realistic topological relationships, and (ii) are limited to random spatial distributions of fracture seeds based on Poisson processes, thereby excluding clustered or regular patterns common in real fracture systems. In the case of heterogeneous rock masses with multiple clustered fracture sets, this leads to an inaccurate representation of connectivity, which significantly impacts the accuracy of hydraulic property estimates and flow modeling results. In addition, the simplified shape of fractures in DFN codes – either rectangular or elliptical, is very different from what observed in our natural sample, where due to mutual abutting relationships the fractures tend to have a triangular or trapezoidal shape, with a strong impact on the evaluation of P32 (i.e. the volumetric fracture intensity), that is a critical parameter in DFN generation. We present a comparative experiment in which a 3D deterministic fracture network was reconstructed from high resolution micro-CT scans of Miocene diatomitic marls (equivalent to the Tripoli Fm., Palena, Central Italy) using a combination of open-source and commercial software, including Move, Petrel, and PZero. This deterministic model was then compared with multiple stochastic DFN realizations sharing the same statistical parameters, generated with DFNWorks, Move and Petrel. Finally, the hydraulic properties of resulting fracture networks and their impacts on flow simulations were assessed using the flow-based model (Petrel), the semi-analytical Oda approach (Petrel and Move) and fully numerical simulations (finite volume in DFNWorks).

Our results indicate that advanced numerical methods, where flow is really simulated along interconnecting fractures, exhibit a greater sensitivity to input data quality than semi-analytical approaches. This discrepancy arises because methods such as the Oda approach rely on idealized assumptions and spatially averaged parameters, disregarding critical parameters such as network topology, connectivity, and fracture aspect ratios. In absence of experiments conducted under controlled lab conditions, we tend to trust the more advanced numerical results (e.g. DFNWorks finite volume) with respect to simplified semi analytical approaches (e.g. Oda).

How to cite: Facci, M., Favaro, S., Casiraghi, S., Agliardi, F., Mittempergher, S., Hussain, W., Hyman, J., Gainov, R., Slipeniuk, O., Fogazzi, M., and Bistacchi, A.: A Comparative Study of Deterministic and Stochastic DFN Models for Rock Mass Hydraulic Property Estimation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18678, https://doi.org/10.5194/egusphere-egu26-18678, 2026.

EGU26-19033 | ECS | Posters on site | ERE5.2

Dating faulting and fluid circulation using the U-Pb carbonate geochronometer reveals Cenozoic reactivation in Gower, Wales 

Nathalie Dawe, Catherine Mottram, Mark Anderson, Billy Andrews, and Matthew Watkinson

With renewed interest in the Bristol Channel and Celtic Sea Basins for geoenergy, South Wales offers the opportunity to study exposed basement rocks at the basin margins. Field relationships show NW-SE and NE-SW trending faults, joints, and fissure fills in South Wales underwent multiple episodes of deformation. Previous studies assume deformation initiated during the Late Variscan, with extensional reactivation during the Mesozoic (e.g. Wright et al., 2009). Recent studies demonstrate the importance of Cenozoic reactivation of Mesozoic structures in the Wessex Basin (Parrish et al., 2018), Bristol Channel Basin (Connolly et al., 2024), and Ireland (Monchal et al., 2023). Due to challenges dating fault rocks associated with low-temperature deformation, the timing of reactivation of Variscan structures is poorly constrained - only one previous study in Gower dates Cretaceous hematite (Ault et al., 2016). New data using the U-Pb carbonate geochronometer at Limeslade Bay, Gower, yields multiple U-Pb ages spanning the Mesozoic to the Cenozoic. A N-S oriented, blocky calcite vein yields a Triassic 206Pb/238U intercept age of 245 ± 11 Ma (MSWD = 2.3, n = 31), and alteration-seam recrystallised host rock yields a Jurassic 206Pb/238U intercept age of 186 ± 19 Ma (MSWD = 2.3, n = 37). Six samples associated with strike-slip deformation yield Eocene-Oligocene (39 - 24 Ma) ages. NW-SE dextral and NE-SW sinistral fault systems displace calcite veins of 27.0 ± 3.4 Ma (MSWD = 1, n = 62) and 24.53 ± 1.28 Ma (MSWD = 1.7, n = 37), respectively. Additionally, an Oligocene (28.6 ± 2.5 Ma, MSWD = 1.2, n = 55) vein is disrupted by Miocene deformation, where a 206Pb/238U intercept age of 13.6 ± 5 Ma (MSWD = 1.4, n = 41) was obtained for recrystallised calcite cross-cutting earlier Oligocene vein fabrics. Cenozoic fault reactivation occurred during N-S compression, resulting from far-field stress during the late Oligocene to Miocene Pyrenean-Alpine orogenies. Fluid circulation is significant in reactivating basin margin structures during basin inversion, which poses a hazard to many geoenergy applications.

 

References:

AULT, A. K., FRENZEL, M., REINERS, P. W., WOODCOCK, N. H. & THOMSON, S. N. 2016. Record of paleofluid circulation in faults revealed by hematite (U-Th)/He and apatite fission-track dating: An example from Gower Peninsula fault fissures, Wales. Lithosphere, 8, 379-385.

CONNOLLY, J., ANDERSON, M., MOTTRAM, C., PRICE, G. & SANDERSON, D. 2024. Using U-Pb carbonate dating to constrain the timing of structural development and reactivation within the Bristol Channel Basin, SW England. Journal of the Geological Society.

MONCHAL, V., DROST, K. & CHEW, D. 2023. Precise U-Pb dating of incremental calcite slickenfiber growth: Evidence for far-field Eocene fold reactivation in Ireland. Geology, 51, 611-615.

PARRISH, R. R., PARRISH, C. M. & LASALLE, S. 2018. Vein calcite dating reveals Pyrenean orogen as cause of Paleogene deformation in southern England. Journal of the Geological Society, 175, 425-442.

WRIGHT, V., WOODCOCK, N. H. & DICKSON, J. A. D. 2009. Fissure fills along faults: Variscan examples from Gower, South Wales. Geological Magazine, 146, 890-902.

How to cite: Dawe, N., Mottram, C., Anderson, M., Andrews, B., and Watkinson, M.: Dating faulting and fluid circulation using the U-Pb carbonate geochronometer reveals Cenozoic reactivation in Gower, Wales, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19033, https://doi.org/10.5194/egusphere-egu26-19033, 2026.

EGU26-20002 | ECS | Posters on site | ERE5.2

Study on mechanism and control of space fracture instability of thick and hard roof under dip angle effect in coal mines 

Xuan Cui, Shengli Yang, and Huiying Zhou

China currently possesses a substantial number of coal seams characterized by thick hard roofs and steep inclinations. With continuous advancements in mining mechanization, increasing mining height and working face length, as well as intensified extraction intensity, the fracture of thick hard roofs induces high-intensity dynamic disturbances and extensive impacts. During weighting periods, intense strata behaviors—such as support crushing, rib spalling, roof collapse, and coal wall spalling—occur frequently. Moreover, the inclination angle of the working face leads to recurrent accidents, including support biting and overturning, severely compromising safe and efficient mining operations. Conventional beam or thin-plate theories are inadequate for analyzing thick hard roofs, as they neglect shear effects induced by roof thickening. The post-fracture structure of thick hard roofs differs significantly from that of thin roofs, resulting in variations in support–surrounding rock interactions and overburden spatial fracture behavior, thereby exacerbating ground control challenges.   To elucidate the disaster mechanisms associated with thick hard roof fracturing and to develop corresponding stability control strategies, this study focuses on the 140502 working face of Kouzidong Coal Mine and the 0448 working face of Chunyi Coal Mine, employing a comprehensive approach that integrates theoretical analysis, numerical modeling, platform development, similar material simulation experiments, rock mechanics testing, and in-situ measurements. The research addresses five key aspects: (1) the law of mine pressure manifestation under thick hard roofs; (2) theoretical analysis of medium-thick plate deformation and failure in roof strata; (3) inclination-thickness coupling effects on roof fracturing; (4) spatial fracture patterns of overburden strata; and (5) support–surrounding rock interactions.

How to cite: Cui, X., Yang, S., and Zhou, H.: Study on mechanism and control of space fracture instability of thick and hard roof under dip angle effect in coal mines, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20002, https://doi.org/10.5194/egusphere-egu26-20002, 2026.

EGU26-20086 | ECS | Posters on site | ERE5.2

Stress-controlled fracture closure and anisotropic flow in carbonate reservoirs: implications for CO₂ storage 

Hager Elattar, Paul W.J. Glover, Richard Collier, and Charlotte Botter

Abstract: Natural fractures exert a first-order control on permeability, sealing capacity, and stress sensitivity of carbonate reservoirs, yet quantitative links between measured fracture-surface roughness and evolving transport properties remain poorly constrained across scales. We present a workflow that combines high-resolution optical surface profilometry with numerical closure and flow modelling to evaluate fracture hydraulic behaviour under effective stress, with implications for CO₂ storage efficiency and containment in fractured carbonates. A 4 × 4 cm fractured carbonate sample is split along the fracture plane to expose complementary surfaces, which are imaged using 3D optical microscopy in the metrology laboratory. Surface height grids are processed in Vision64 and exported for analysis. We computed roughness statistics and constructed aperture fields by digitally pairing the two surfaces, thereby enabling progressive mechanical closure to be simulated as either a prescribed displacement (closure) or field-stress-controlled loading.

Using closure-dependent aperture maps, we quantified transport anisotropy by solving pressure-driven flow through the fracture for orthogonal directions. Conductivity/permeability proxies are calculated using both cubic-law scaling and a spatially variable conductivity formulation (k ∝ b³) solved on the aperture grid. In parallel, capillary entry pressure is estimated from aperture distributions to evaluate stress-dependent sealing. Results show a nonlinear reduction in connected aperture with increasing closure, producing rapid declines in fracture conductivity and increases in capillary entry pressures as contact patches expand and percolating pathways collapse. Directional differences in flow and sealing metrics reveal pronounced anisotropy inherited from the surface topography, with dominant flow aligned with the most persistent connected channels.

Finally, stress-path sweeps (injection/depletion and shear ramp scenarios) demonstrate how effective normal stress and shear-related dilation can produce contrasting permeability–capillary responses, highlighting the potential for hysteresis and path dependence during CO₂ injection and pressure cycling. This integrated approach provides a quantitative bridge between laboratory-scale roughness measurements and stress-sensitive fracture transport, supporting improved parameterisation of fractured carbonate reservoirs in CO₂ storage models and risk assessment for leakage versus immobilisation.

Keywords: capillary entry pressure, fracture roughness, CO₂ storage integrity, anisotropy.

 

How to cite: Elattar, H., Glover, P. W. J., Collier, R., and Botter, C.: Stress-controlled fracture closure and anisotropic flow in carbonate reservoirs: implications for CO₂ storage, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20086, https://doi.org/10.5194/egusphere-egu26-20086, 2026.

EGU26-20517 | ECS | Posters on site | ERE5.2

An experimental study of fault growth in a 2D Biaxial apparatus 

Sakshi Yadav, Axelle Amon, Giovanni Camanni, Giacomo Russo, Enza Vitale, and David Iacopini

Placing constraints on the geometry and growth of faults has significant implications for the management of resources in the subsurface; faults are widespread structures and can either compartmentalise subsurface reservoirs or provide favourable fluid migration pathways.

There are two widely accepted models of fault growth: the isolated fault growth model and the constant length fault growth model. These models, largely derived from field, seismic, and analogue modelling data, both describe three stages in fault growth: (1) propagation of fault segments, (2) slip accumulation on fault segments, and (3) segment interaction and linkage. However, they differ in how the initial fault segments interact, whether they are kinematically dependent, and how rapidly their full length is established. The debate is currently still open on which model best describes natural faults, and what geological controls favor one model over the other.

To further address the topic of fault growth, we investigate the different stages of growth through two sets of experiments. First, loading experiments are performed on intact samples of a rock analogue material to track both the propagation of the fracture and the displacement accumulation to test which of the two fault growth models most accurately describes the initial stages of fault propagation. Second, loading experiments are performed on samples with pre-cuts to replicate realistic fault segment geometries, to track fault tip migration and displacement partitioning during the linkage stage of fault growth, to test geometrical controls on the process of fault linkage.

The samples are made of a rock analogue material capable of accommodating displacement gradients through ductile processes, similar to those observed in natural rocks over geological timescales. This material is cohesive and allows the creation of pre-cuts to replicate fault segment geometries. Loading experiments are conducted in a biaxial apparatus at low strain rates, coupled with an interferometric technique using an optical bench to obtain speckle patterns. These speckles are employed to track in high resolution the increase in the length of the fault using Diffusive Wave Spectroscopy (DWS). In addition, we concurrently use the same speckle patterns to track displacement along the fault using Digital Image Correlation.

How to cite: Yadav, S., Amon, A., Camanni, G., Russo, G., Vitale, E., and Iacopini, D.: An experimental study of fault growth in a 2D Biaxial apparatus, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20517, https://doi.org/10.5194/egusphere-egu26-20517, 2026.

EGU26-21242 | Posters on site | ERE5.2

Velocity-dependent frictional properties of fault gouges in the Upper Rhine Graben under hydrothermal conditions: Implications for induced seismicity 

Tesfay Kiros Mebrahtu, Michael Rudolf, André Niemeijer, Virginia Toy, Laurence Warr, and Andreas Henk

The Upper Rhine Graben (URG) is a tectonically active area that has been extensively investigated for its geothermal energy potential. However, modification of fluid pressures in subsurface reservoir for geothermal energy production can affect the regional stress field inducing seismicity that causes high public and social concern as well as economic losses, e.g., in Landau, Insheim, Soultz-sous-Fôrets, Rittershofen, Strasbourg, and Basel. The effective frictional strength and stability of faults depend on the nature of stimulation, the reservoir conditions, and subsurface fault rock characteristics. It is crucial that we explore the complex relationships between these factors and the frictional stability of faults for safe geothermal energy operations. In this study, to understand the seismic potential of faults in geothermal reservoir rocks, we investigated how the frictional behaviour of fault gouges from the URG area varies when stimulated with fluids at different temperatures and pressures using hydrothermal rotary shear friction experiments.

Our data are fit by rate-and-state friction laws (RSF) and the mechanical results are supplemented with microstructural observations to identify the active deformation mechanisms. We also analyzed porosity, grain size, shape, and mineralogy of fault gouges employing scanning electron microscopy and energy-dispersive spectroscopy. Simulated fault gouges were prepared from Muschelkalk, Buntsandstein, Rotliegend, and crystalline basement rocks (granite and gneiss), and velocity-stepping tests were conducted at temperatures from 20 to 250 ºC, effective normal stresses of 60 and 75 MPa, pore fluid pressures of 40 and 50 MPa, and slip velocities 0.3 to 100 µm/s, depending on the fault gouge type. Moreover, X-ray diffraction (XRD) was performed on the fault gouge samples to determine their mineralogical composition, which significantly influences the mechanical behavior of the gouges.

We observed differences in gouge sliding strength and frictional character as a function of both sliding velocity and temperature. Preliminary mechanical results show a strong temperature dependent steady-state strength during initial sliding, with friction coefficients in the range of 0.38 – 0.9. All the fault gouges exhibit stable velocity-strengthening (aseismic) behavior, except those derived from Rotliegend and granite, which show a transition from velocity strengthening to velocity weakening with increasing sliding velocity at T>200 ºC. The rate-and-state parameters (a, b, and Dc) for Rotliegend and granite show a transition from a velocity-neutral to velocity- and strain-weakening behavior at temperatures between 200 and 250 ºC. This transition enhances mechanical instability and creates conditions more favorable for earthquake nucleation. In contrast, the Muschelkalk and Buntsandstein samples revealed velocity-strengthening and strain-hardening behavior, favouring aseismic creep over dynamic rupture, which we interpret to be mainly due to the presence of small amounts of weak hydrous minerals and amorphous content. These results indicate that the Rotliegend and crystalline basement rocks (granite) are more prone to induced seismicity than Muschelkalk and Buntsandstein. Our findings provide vital insights into the understanding of fault behavior at regional scales, allowing constraint input for seismic models, and strengthen the connection to numerical models.

How to cite: Mebrahtu, T. K., Rudolf, M., Niemeijer, A., Toy, V., Warr, L., and Henk, A.: Velocity-dependent frictional properties of fault gouges in the Upper Rhine Graben under hydrothermal conditions: Implications for induced seismicity, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21242, https://doi.org/10.5194/egusphere-egu26-21242, 2026.

EMRP2 – Geomagnetism

This work presents a new method for interpreting potential geomagnetic field data. It combines the analytical signal method, which is independent of the direction of magnetization, with the two-dimensional continuous shearlet transform (CST). First, the dominant directions of the structural geological features of a given area are estimated using geological data and conventional interpretation methods such as horizontal gradient, Euler deconvolution and wavelet transform. These directions are then used to determine the shearing parameters required for the shearlet transform calculation. The two-dimensional CST is then applied to the amplitude of the analytical signal calculated from potential geomagnetic anomaly field data. Mapped maximas of the amplitude of the shearlet transform for the full range of CST scales enable identification of geological discontinuities. The proposed approach avoids reduction to the pole (RTP), which is often problematic in areas with high remanence. It also effectively attenuates the random noise associated with the analytical signal, thereby improving the mapping of magnetic anomalies. Furthermore, it facilitates structural interpretation in geologically complex environments. This process is particularly useful in mining, oil, and geothermal exploration, representing a significant advance in geomagnetic data interpretation.

How to cite: Ouadfeul, S.-A.: Potential geomagnetic field data interpretation using the analytical signal and the two-dimensional continuous Shearlet transform., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-300, https://doi.org/10.5194/egusphere-egu26-300, 2026.

The Assarag region is located in the northern part of the Ouzellagh-Siroua salient, being a segment of the central
Anti-Atlas basement bulging within the High-Atlas Belt of Morocco. It consists mainly of the Late Ediacaran
Magmatic Suites (LEMS) of the Ouarzazate Group (580-539 Ma). The LEMS comprise high potassic calc-alkalic I type
granitoids that host the Imourkhssen Cu-Mo-Au-Ag porphyry mineralization. The aeromagnetic data from
the Assarag region led to describe structural features in the LEMS based on their magnetic footprints. aeromagnetic
datasets were processed using several transformations including the reduction to pole (RTP), Upward
continuation (UC), Tilt derivative (TD), Center for Exploration Targeting (CET) and Euler deconvolution (ED)
filters. RTP, TD and CET transformations allowed to map NNE-SSW, NNW-SSE and NE-SW trending faults in the
north, in addition to a curved magnetic halo in the southwestern part of the Assarag area. The UC filter subdivided
the Assarag area into two magnetic morpho-structural domains: a northern region with low-magnetic
features, and a southern high-magnetic region with positive curved trending patterns. The ED results match
and support the extracted lineaments. The aeromagnetic data were also processed by a 2D Spatio-Spectral
Feature Extraction and Selection tool (SFES2D) using two-dimensional continuous wavelet transformations
(2D CWT), principal component analysis (PCA) and independent component analysis by kurtosis and negentropy
methods (k-ICA and n-ICA). The PCA results corroborate previously extracted lineaments and highlight a new
ENE-WSW oriented structure. Meanwhile, the CWT allowed us to conclude that NNE, NNW and NE trends are
shallow and emphasized deep NW-SE and ENE-WSW structures in the southern part of the Assarag area. ICA
emphasizes the ENE lineament and matches the previous results. We herein define the deeper ENE trend as a part
of the South Atlas Fault (SAF), which crosscuts the LEMS in the study area. Meanwhile, the shallow NE-SW and
NNE-SSW tectonic features likely served as conduits for the ore-bearing fluids, leading to the Imourkhssen Cu-
Mo-Au-Ag mineralization. Consequently, these directions present a valuable approach for guiding mineral
exploration in the Ouzellagh-Siroua salient, from prospect to regional scales.

How to cite: Ferraq, M., Belkacim, S., Cheng, L.-Z., and Abbassi, B.: Aeromagnetic data from the Assarag area (Ouzellagh-Siroua salient, central Anti-Atlas, Morocco): Implications for the Imourkhssen porphyry mineralization, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-450, https://doi.org/10.5194/egusphere-egu26-450, 2026.

This study presents a fully automatic inversion technique for interpreting magnetic anomalies of two-dimensional (2D) listric fault structures with arbitrary magnetisation. Listric faults exhibit curved geometries with steep dips near the surface that decrease with depth. But most studies assume a planar fault geometry to the listric faults, which is rarely valid in reality. Accurately modelling such structures is essential because many sedimentary basins and extensional tectonic settings contain listric faults that significantly influence subsurface geometry. Forward modelling is performed using the equation derived by Ani Nibisha et al. (2021), that computes magnetic anomalies of listric faults in any component (vertical, horizontal, or total), with arbitrary magnetisation directions by incorporating both induced and remanent magnetic components. In the proposed method, polynomial function of arbitrary degree is used to represent the nonplanar fault surface. The coefficients of these polynomials, with structural parameters like depths to the top and bottom of the fault, location of the fault edge, and magnetisation intensity and direction, are estimated directly from the magnetic anomaly profile. The inversion uses Marquardt’s (1970) algorithm for optimisation. With a vertical step approximation, the initial parameters are generated automatically based on certain characteristic anomaly features like maximum and minimum anomaly points, and are updated iteratively until a predefined convergence criterion is satisfied. The misfit between observed and calculated anomalies guides model updates, and the method adaptively adjusts the damping factor to ensure stable convergence. The validity and robustness of the inversion technique are demonstrated through two examples. In the synthetic test, a fifth-degree polynomial is used to describe the fault geometry, and Gaussian noise is added to the computed anomalies for a realistic approach. The inversion successfully reconstructs the geometry, magnetisation intensity, and direction, even when lower-order polynomials (second or third degree) are used, since the optimal degree to define the fault geometry remains unknown with the absence of apriori information about the subsurface during inversion. This demonstrates that the technique can produce geologically reasonable solutions even without precise prior knowledge of the fault’s curvature. This technique is compared with the inversion technique by Murthy et al. (2001), which assumes planar fault surfaces and shows that such simplified models fail to recover realistic structures for listric faults. The method is further applied to real total-field magnetic anomalies from the western margin of the Perth Basin, Australia, which is known for hydrocarbon prospectivity and characterised by deep, curved normal faults. Using a second-degree polynomial, the technique identifies a listric fault with its top near 4 km depth and bottom near 14.8 km, yielding a close fit to observed anomalies with small residuals. The recovered geometry aligns well with seismic observations that reveals the listric nature of the fault (Middleton et al. 1993), reinforcing the reliability of the inversion approach. In contrast, inversion assuming a planar fault plane produces geologically inconsistent results. In conclusion, this technique improves the interpretation of magnetic datasets in regions dominated by extensional tectonics and curved fault structures, offering more realistic subsurface models than traditional planar-fault methods.

How to cite: Nibisha, A. and Vishnubhotla, C.: Interpretation of Magnetic Anomalies of 2D Listric Faults with arbitrary magnetisation: A Polynomial-Based Automatic Inversion Approach, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1015, https://doi.org/10.5194/egusphere-egu26-1015, 2026.

EGU26-1487 | Orals | EMRP2.2

Gravity from exploration to field management 

Vijay P Dimri and Ravi Prakash Srivastava

Gravity surveys are well known for the exploration of frontier basins and understanding of the crustal structures.  Recent advances in gravity instrumentation along with processing and interpretation techniques have significantly improved the accuracy of the gravity surveys. The increased accuracy of the gravity measurements has led to Time Lapse gravity (also known as 4D gravity) monitoring of the Oil/Gas fields, where repeatability of the various gravity surveys at different time intervals are crucial.

Plan is to showcase two examples, one related optimum gridding of land 2-D gravity survey based on the scaling concept from Vindhayan basin of India and another where gravity is efficiently used in a very cost effective way for the field management based on repeated gravity measurements at seafloor (Time Lapse gravity) for subsidence and fluid movement monitoring in North sea.

How to cite: Dimri, V. P. and Srivastava, R. P.: Gravity from exploration to field management, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1487, https://doi.org/10.5194/egusphere-egu26-1487, 2026.

EGU26-3131 | Posters on site | EMRP2.2

Gravimetry across spatial scales – how powerful is gravity? 

Hans-Jürgen Götze and Denis Anikiev

Gravity is a fundamental geophysical method that provides unique insight into subsurface density variations. Its sensitivity spans an exceptional range of spatial scales, from centimetre-scale laboratory experiments and borehole measurements to continental - and global-scale satellite observations. Despite its long-standing application, the practical limits and resolving power of gravimetry across these scales are still not widely appreciated. At regional to global scales, satellite missions such as GRACE and GOCE have transformed our understanding of mass redistribution within the Earth system. They enable the monitoring of ice mass loss, hydrological change, and large-scale mantle processes, achieving microgal (10⁻⁸ m s⁻²) accuracy with spatial resolutions of several hundred kilometres. These capabilities demonstrate gravimetry’s strength in detecting large-scale density anomalies and temporal mass transport. At crustal and reservoir scales, terrestrial and airborne gravity measurements resolve subtle variations related to geological structures, sedimentary basins, and fluid movements. Advanced data processing- such as terrain, Bouguer, and isostatic corrections- improves signal fidelity, while time-lapse relative gravimetry can detect changes associated with e.g. volcanic unrest, groundwater depletion, and reservoir dynamics down to the sub-microgal level. At the smallest scales, absolute gravimeters and emerging quantum sensors push precision further, enabling laboratory-based density determinations and environmental monitoring with unprecedented stability. Increasing resolution, however, introduces challenges related to topographic effects, instrumental drift, and signal ambiguity, requiring robust modelling and/or inversion strategies, and integration with complementary geophysical data. We review representative applications across satellite, regional, and local domains, quantify achievable spatial and temporal resolution, and discuss future perspectives, joint interpretation with magnetic and seismic methods, and the growing role of artificial intelligence in gravity data analysis.

How to cite: Götze, H.-J. and Anikiev, D.: Gravimetry across spatial scales – how powerful is gravity?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3131, https://doi.org/10.5194/egusphere-egu26-3131, 2026.

EGU26-3376 | ECS | Orals | EMRP2.2

High-resolution magnetic, sidescan, and water column constraints on the tectono-magmatic and hydrothermal evolution of Healy submarine volcano, Kermadec arc, New Zealand 

Alessio Bagnasco, Fabio Caratori Tontini, Cornel E. J. de Ronde, Sharon L. Walker, Luca Cocchi, Alessandro Ghirotto, and Egidio Armadillo

Here we present a multidisciplinary, high-resolution investigation of Healy submarine volcano, located in the southern Kermadec arc, New Zealand, combining magnetic, sidescan, and hydrothermal plume datasets to constrain the structure and evolution of its magmatic–hydrothermal system.

Near-seafloor magnetic and sidescan sonar data acquired by the Autonomous Underwater Vehicle (AUV) Sentry have been integrated with shipborne magnetic and gravity measurements, multibeam bathymetry, acoustic backscatter, and hydrothermal plume observations, as well as seafloor imagery and in situ temperature measurements collected by the Pisces V submersible, to develop a detailed geological and geophysical characterization of the volcano.

High-resolution sidescan sonar data reveal fine-scale volcanic and tectonic structures, including lava flow textures, fracture networks, and cone morphology providing context for interpreting magnetic anomalies and hydrothermal plume results. Magnetic ‘lows’ are spatially associated with older, caldera-related structures and demarcate zones of ancient hydrothermal discharge, consistent with the loss of magnetite due to hydrothermal alteration. By contrast, younger basaltic cones emplaced along NNE–SSW-trending lineaments exhibit relatively high magnetization signatures and host the currently active hydrothermal venting, characterized by directly observed low-temperature discharge, while hydrothermal plume data (e.g. turbidity anomalies) suggest the possible presence of higher-temperature venting. Taken together, the spatial distribution of volcanic facies, structural lineaments, magnetization patterns, and hydrothermal activity suggests a temporal evolution in magma emplacement and fluid pathways. This evolution is consistent with a transition from caldera-related, arc-dominated volcanism toward more localized basaltic magmatism exploiting extensional structures, which may reflect the early development of back-arc extension.

Our results highlight the important role of multi-sensor, high-resolution surveys in developing robust conceptual models of submarine volcanic systems, and demonstrate how combined gravity, magnetic, sidescan, and hydrothermal plume investigations are prerequisites for understanding hydrothermal processes and related resources in remote deep-sea environments.

How to cite: Bagnasco, A., Caratori Tontini, F., E. J. de Ronde, C., L. Walker, S., Cocchi, L., Ghirotto, A., and Armadillo, E.: High-resolution magnetic, sidescan, and water column constraints on the tectono-magmatic and hydrothermal evolution of Healy submarine volcano, Kermadec arc, New Zealand, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3376, https://doi.org/10.5194/egusphere-egu26-3376, 2026.

High resolution magnetic surveys of the seafloor have become more ubiquitous in recent times with the broad application of autonomous underwater vehicles (AUV) to seafloor investigation.  AUVs can follow a precise path repeatedly which allows to the possibility of repeated measurements through time. This provides unique insight in what was considered mostly static seafloor magnetic properties. Some examples of dynamic magnetic field include anomalies associated with recent lavas cooling and becoming magnetized, while deep-seated thermal anomalies associated with magma chambers may demagnetize the overlying crust and create a detectable signal at the seafloor if not the sea surface.  We present an update to a temporal magnetic study of Axial seamount in the northeast pacific.  Axial Seamount is active having erupted in 2015, 2011, and 1998. Axial is part of the Ocean Observatory Initiative Regional Cabled Array.  Magnetic field is not monitored but repeat, semi-yearly surveys have been done by AUV Sentry for geodetic purposes which happily also collects magnetic field data. We present recent 2024 results from Axial Seamount as it inflates for a future eruption.

How to cite: Tivey, M.: Temporal Magnetic Surveys using Autonomous Underwater Vehicles, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3598, https://doi.org/10.5194/egusphere-egu26-3598, 2026.

EGU26-6661 | Posters on site | EMRP2.2

Potential field and structural control of a Sn-W rich area, W Iberia (Central Iberian Zone) 

Puy Ayarza, Manuela Durán, Pablo Calvín, Irene DeFelipe, Laura Yenes, Alberto Santamaria, Imma Palomeras, Yolanda Sanchez Sanchez, Mariano Yenes, Ramon Carbonell, and Juan Gomez Barreiro

The Sn-W belt of western Iberia coincides with large-scale magnetic anomalies, namely the Porto-Veira-Guarda and the Central System Magnetic Anomalies (PVGMA and CSMA) challenging the well-known relationship between Sn ores and ilmenite (non-magnetic) granites. In fact, these magnetic anomalies overlap a series of gneiss domes developed in the latest stages of Variscan evolution and often hosting local, but abundant critical mineral ores.  Paradoxically, these domes are cored by non-magnetic granites and their by-products, rising the question about the source of the magnetism.

With the goal of unravelling the relationship between mineralization, tectonics and magnetic anomalies, we have carried out a 50 x 50 km2 ground potential field survey in the Martinamor Gneiss Dome and its surroundings, to the southwest of Salamanca. Results from analytical processing and modelling show that shallow and local magnetic anomalies respond to the existence of highly magnetic, albeit uncommon, Upper-Proterozoic to Ordovician metasediments that are not related to the younger (338-300 Ma) Sn-W mineralization. Contrarily, the ores appear at the non-magnetic core of the dome and are frequently related to high gradient zones within potential field data. The latter coincide with the location of extensional detachments that must have acted as pathways for mineralizing fluids. To the southwest of the study area and at higher depths, conspicuous magnetic maxima coincide with Bouguer gravity anomaly maxima and with high shear-wave velocity anomalies, pointing out to the existence of non-outcropping mafic rocks. These lithologies might be progressively more common at depth and be the source of the long wavelength PVGMA and CSMA.  

The present dataset indicates that, as it has been generally acknowledged, magnetic rocks do not host Sn (and W) mineralization but regardless of this evidence, in western Iberia, there might be a common mechanism that triggers mineralization and magnetization. Constraining the age of the latter is key to further interpret this area.

This research has been funded by project SA066P24 from the JCYL

How to cite: Ayarza, P., Durán, M., Calvín, P., DeFelipe, I., Yenes, L., Santamaria, A., Palomeras, I., Sanchez Sanchez, Y., Yenes, M., Carbonell, R., and Gomez Barreiro, J.: Potential field and structural control of a Sn-W rich area, W Iberia (Central Iberian Zone), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6661, https://doi.org/10.5194/egusphere-egu26-6661, 2026.

EGU26-7486 | ECS | Posters on site | EMRP2.2

Inversion of gravity and magnetic data in the presence of topography using deformable hexahedral elements 

Lahcene Bellounis, Romain Brossier, Ludovic Métivier, Claire Bouligand, and Stéphane Garambois

Potential-field geophysical data are commonly used to image geological structures in areas characterized by strong topographic variations, such as volcanic and rift systems. However, the forward modelling of potential-field data using traditional approaches may inadequately represent strongly varying topography if the physical space is not discretized appropriately, potentially biasing inversion results and subsequent geological interpretations. Recent modeling strategies, such as the use of numerical integration schemes within deformable hexahedral elements coupled with an algorithm for local refinement of the forward modeling mesh, have been shown to improve the modeling accuracy while maintaining a reasonable computational cost [Bellounis et al., Geophys. J. Int., ggag009, 2026]. Building on this previous work, we present the implementation of an inversion framework that is consistent with this numerical approach and assess its performance using a series of synthetic data that have not been corrected for topographic effects. The inversion is performed on models discretized using deformable hexahedral elements where physical properties are represented by 2nd order polynomials defined by their values at grid nodes. We first validate the inversion scheme using a model without topography, before considering a second example that incorporates complex topographic variations representative of the Krafla geothermal system in northern Iceland. These synthetic experiments highlight the challenges introduced by topography in the inversion process and demonstrate the improved integration of topographic information enabled by the proposed discretization and inversion strategy. We further examine the influence of the inverse problem regularization parameters on the recovery of subsurface anomalies, thereby providing insights into the advantages and current limitations of the newly implemented inversion framework.

How to cite: Bellounis, L., Brossier, R., Métivier, L., Bouligand, C., and Garambois, S.: Inversion of gravity and magnetic data in the presence of topography using deformable hexahedral elements, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7486, https://doi.org/10.5194/egusphere-egu26-7486, 2026.

EGU26-8366 | ECS | Posters on site | EMRP2.2

Open-source gravity and magnetic forward model of ellipsoids 

Santiago Soler, Kelly Baker, and Lindsey Heagy

Analytic solutions for the gravitational potential of a homogeneous ellipsoid have existed since the first half of the nineteenth century, while analytic solutions for the magnetic field were developed by the end of the same century. The existence of such analytic solutions allowed geophysicists to use ellipsoidal bodies to approximate complex geological structures and model their respective gravity and magnetic fields. Ellipsoids are of particular interest for modelling ore bodies and structures with high magnetic susceptibilities, since they are the only geometric bodies with analytic solutions for their magnetic field that account for self-demagnetization effects. Nonetheless, modern, easy-to-use, up-to-date, and open-source implementations of these analytic solutions are scarce if non-existent.

We present an open-source Python implementation of the analytic solutions of the gravity acceleration and magnetic field generated by homogeneous ellipsoids with arbitrary rotations. This new code allows users to easily define ellipsoids by their semi-axes lengths, the coordinates of their geometric centers, and three rotation angles. The gravity acceleration and magnetic field they generate can be computed on any point in space, including internal and external points to the bodies, through specific functions for each field. The code supports triaxial, prolate and oblate ellipsoids, including spheres. Users can assign physical properties to each ellipsoid, like its mass density, magnetic susceptibility, and remanent magnetization. The magnetic susceptibility can be a single value for isotropic susceptibility, or a second-order tensor to account for anisotropy. The total magnetization of the ellipsoid is obtained as a combination of the induced and remanent magnetization, accounting for self-demagnetization effects.

This implementation can be used to predict the gravity and magnetic field of any set of ellipsoids for hypothesis testing, survey designing, and stochastic inversions. In future work, we plan to include analytic derivatives of the fields with respect to ellipsoid's parameters, so the code can also be used for deterministic inversions.

The ellipsoid class and their forward modelling functions have been included in Harmonica: an open-source Python package for processing and modelling gravity and magnetic data, part of the Fatiando a Terra project. We followed best practices for its development, including thorough testing and extensive documentation, leading to a robust, well-designed, and well-tested implementation of such analytic solutions.

How to cite: Soler, S., Baker, K., and Heagy, L.: Open-source gravity and magnetic forward model of ellipsoids, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8366, https://doi.org/10.5194/egusphere-egu26-8366, 2026.

Mapping crustal thermal structure is fundamental to studies of lithospheric rheology, tectonic evolution, and deep geothermal resource assessment. Curie point depth (CPD) estimates derived from magnetic anomalies are commonly used to infer geothermal gradients, but many approaches remain sensitive to simplifying assumptions about magnetization. Here, a computationally efficient, spatial-domain framework is developed to invert CPD topography by representing the CPD as an effective magnetization-contrast interface and computing its magnetic response using Cauchy-type surface integrals. This formulation replaces three-dimensional volume integration with a two-dimensional surface integral while preserving the governing potential-field physics, which facilitates high-resolution forward modelling and regularized interface inversion. Synthetic experiments are conducted to evaluate numerical accuracy and inversion robustness. The method is applied to magnetic anomalies over the Gonghe Basin on the northeastern Tibetan Plateau, a high-temperature geothermal region. The inverted CPD is interpreted as an effective magnetic-thermal boundary conditional on the assumed susceptibility model, and is compared with results from spectral techniques, equivalent-source reconstructions. Finally, the CPD constraints are integrated with independent geophysical and geological information to construct a three-dimensional temperature model of the Gonghe Basin, which provides quantitative insight into the distribution of thermal anomalies and the likely heat-source characteristics and driving mechanisms.

How to cite: Sun, J. and Liu, S.: Curie Point Depth Inversion From Magnetic Data Using a Cauchy-type Integral Interface Framework: Application to the Gonghe Basin (northwest China), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8781, https://doi.org/10.5194/egusphere-egu26-8781, 2026.

EGU26-9535 | Posters on site | EMRP2.2

The magnetic and electromagnetic integrated geophysical investigation of the Weilasituo tin polymetallic deposit, Inner Mongolia, China 

Shuang Liu, Ronghua Peng, Bo Han, Yajun Liu, Tao Yang, and Zhenhua Zhou

The Weilastuo tin polymetallic deposit is located in the central-southern segment of the Great Xing’an Range, which is an important metallogenic belt of northern China. The Quaternary is widely distributed in the ore district, with the host rocks primarily consisting of migmatitic gneisses and a small amount of Carboniferous quartz diorite. The ore-related intrusive bodies are concealed at depths within the tin-zinc ore district, with the shallowest occurrences reaching approximately 400m below the surface. This study collected the rock samples from the Weilastuo and other districts, and accurately measured the physical properties parameters including resistivity, polarization, magnetic susceptibility, and natural remanent magnetization for over 480 rock samples. The research conducted multi-geophysical explorations and methodological experiments in the Weilastuo ore district, including surface and airborne magnetic exploration, audio magnetotellurics (AMT), and transient electromagnetic (TEM). The 3D magnetic susceptibility and resistivity structure model of the Weilastuo ore district were constructed, providing geophysical constraints for developing geophysical exploration models for shallow cover polymetallic tin deposits of Inner Mongolia, China. This study was supported by project grant no. 2024ZD1001502.

How to cite: Liu, S., Peng, R., Han, B., Liu, Y., Yang, T., and Zhou, Z.: The magnetic and electromagnetic integrated geophysical investigation of the Weilasituo tin polymetallic deposit, Inner Mongolia, China, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9535, https://doi.org/10.5194/egusphere-egu26-9535, 2026.

EGU26-11430 | ECS | Orals | EMRP2.2

From Sharp to Diffuse: How Erosion Level Controls the Architecture of Continental Sutures in the Crust 

Mateusz Mikołajczak, Stanisław Mazur, Randell Stephenson, Christian Schiffer, Piotr Krzywiec, and Jarosław Majka

Continental sutures are fundamental markers of past plate convergence, yet their geological expression varies markedly depending on erosion level and crustal depth. Classical descriptions of sutures emphasize narrow, localized zones characterized by ophiolites, mélanges, arc-related assemblages, and high-pressure metamorphic rocks, often exposed at the surface. However, such features typically reflect shallow-crustal levels of preservation. Here we demonstrate that deeply eroded or buried sutures may lack this diagnostic surface expression and instead form wide, diffuse boundary zones within the middle and lower crust, extending laterally for 100–200 km. This conceptual framework is illustrated with two contrasting examples from Europe: the early Palaeozoic suture between Baltica and Avalonia and the Paleoproterozoic suture between Fennoscandia and Sarmatia within the East European Craton.

The first case examines the German–Polish Caledonides and the Thor Suture separating Avalonia from Baltica. Integration of geological data with reinterpretation of the Basin-9601 deep seismic profile, complemented by newly constructed 2-D forward gravity modelling and regional gravity and magnetic compilations, allows refinement of the crustal architecture across eastern Germany and western Poland. The Caledonian Deformation Front is shown to mark the northern limit of a thin-skinned fold-and-thrust belt, composed of Ordovician metasediments derived from a Caledonian accretionary wedge near Rügen and of deformed foreland-basin sediments incorporated into the orogenic wedge farther east. In contrast, the Thor Suture itself—defined as the thrust of Avalonia’s crystalline basement over Baltica—is located ~120 km farther south, beneath the depocentre of the North German Basin and along the Dolsk Fault Zone in western Poland. At depth, the lower crust of Baltica is underthrust southward to the Flechtingen High and toward the Variscan Rheno–Hercynian suture. This geometry demonstrates that, although the Caledonian suture has a narrow and classical expression in the shallow crust, it broadens downward into a wide lithospheric-scale transition zone, coinciding with mantle lithosphere necking between thick Baltican and thinner Avalonian lithosphere.

The second example addresses the Paleoproterozoic Fennoscandia–Sarmatia Suture (FSS) in eastern Poland. Reassessment of deep reflection seismic data from the PolandSPAN™ survey, combined with 2-D gravity and magnetic modelling and 3-D models of basement depth and crustal thickness, reveals a fundamentally different suture style. Rather than a discrete fault, the FSS is expressed as a 100–120 km wide transitional zone involving the Belarus–Podlasie Granulite Belt and the Okolovo Belt. These domains are characterized by anomalously dense and magnetically susceptible lithologies, interpreted as remnants of arc-related magmatic complexes, mafic igneous suites, and high-pressure metamorphic rocks. Seismic and potential-field data demonstrate that these features continue through the entire crust, indicating a deeply rooted Paleoproterozoic collision that has been subsequently overprinted but not obliterated.

Together, these examples show that sutures preserved at shallow levels are narrow and lithologically distinctive, whereas deeply eroded or ancient sutures are cryptic, broad, and best recognized through integrated seismic and potential-field analyses. At the same time, we acknowledge that differences in Precambrian versus Phanerozoic tectonic regimes—such as lithospheric strength, thermal structure, and strain distribution—may further contribute to the development of especially wide deformation zones in Palaeoproterozoic sutures.

How to cite: Mikołajczak, M., Mazur, S., Stephenson, R., Schiffer, C., Krzywiec, P., and Majka, J.: From Sharp to Diffuse: How Erosion Level Controls the Architecture of Continental Sutures in the Crust, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11430, https://doi.org/10.5194/egusphere-egu26-11430, 2026.

EGU26-11655 | ECS | Posters on site | EMRP2.2

Enhanced Antarctic geothermal heat flow derived from defractal spectral analysis of aeromagnetic data: examples from the Thwaites Glacier and Dome C regions 

Shi Quan Ooi, Fausto Ferraccioli, Pietro Latorraca, Jonathan Ford, Ben Mather, Egidio Armadillo, Joerg Ebbing, Graeme Eagles, Karsten Gohl, Javier Fullea, Massimo Verdoya, and Chris Green

Antarctic geothermal heat flow (GHF) is one of the least constrained basal boundary conditions affecting subglacial hydrology and ice sheet dynamics. Furthermore, the paucity of knowledge about GHF hampers our understanding of the linkages between geodynamic evolution and tectono-thermal conditions in Antarctica.

Here we present the results of enhanced spectral analysis of a new Antarctic aeromagnetic anomaly compilation, conformed at long wavelengths with SWARM satellite magnetic data. We apply manual picking of defractal magnetic power spectra on several different major subglacial lake districts in both West and East Antarctica and compare our results with those obtained using automated workflows implemented in PyCurious. Furthermore, we compare our results with independent GHF estimates from seismology, multivariate-similarity approaches and previous magnetic studies.

We show that in the Amundsen Sea Embayment in West Antarctica manual spectral picking resolves the spatial heterogeneity in GHF anomalies better than automated approaches. We newly define a wide coastal region of relatively lower values corresponding to recently inferred mafic intrusions within this sector of the West Antarctic Rift System and higher GHF in the Byrd Subglacial Basin. This is highly significant as it suggests that elevated GHF may contribute to the onset of enhanced ice flow in the interior of the Thwaites Glacier catchment. Additionally, we find localised GHF anomalies in the area of the Thwaites active lakes that may affect subglacial water availability and promote reduced basal shear stress despite the widespread hard bed conditions related to the occurrence of predominantly crystalline rocks.

In East Antarctica, the manual approach confirms the existence of elevated GHF beneath the Dome C subglacial lake district. However, the anomaly is more linear than previously recognised and better aligned with the trend of major aeromagnetic anomalies interpreted as reflecting extensive Paleo to Mesoproterozoic basement in the sector of East Antarctica. Notably, remarkably similar magnetic anomalies are imaged in formerly contiguous Australia where highly radiogenic igneous provinces significantly enhance GHF.

Overall, we find that the choice of appropriate window sizes and spectral ranges coupled with careful inspection of individual power spectra (including the recognition of outliers) and the choice of defractal parameters is important to better define regional scale heterogeneity in Curie Depth estimates. We also find that incorporating the results of independent seismic, multivariate approaches, and expert knowledge in the geological settings of the different study regions is beneficial to better define the realistic ranges of average Curie Depth and for the conversion from Curie Depth to GHF.

The results of our magnetic studies need to be integrated into thermal modelling frameworks together with the evolving knowledge of crustal and lithospheric properties in Antarctica, including intracrustal heat production and sedimentary basin distribution. This approach will yield improved spatial resolution and accuracy of Antarctic GHF and better understanding of the geological origin and significance of major GHF anomalies.

How to cite: Ooi, S. Q., Ferraccioli, F., Latorraca, P., Ford, J., Mather, B., Armadillo, E., Ebbing, J., Eagles, G., Gohl, K., Fullea, J., Verdoya, M., and Green, C.: Enhanced Antarctic geothermal heat flow derived from defractal spectral analysis of aeromagnetic data: examples from the Thwaites Glacier and Dome C regions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11655, https://doi.org/10.5194/egusphere-egu26-11655, 2026.

EGU26-12390 | Posters on site | EMRP2.2

A Deep Learning Framework for Joint Inversion of Gravity and Magnetic Data 

Xingjian Yan, Shuang Liu, and Mengzhi Lv

Data-driven deep learning inversion of gravity and magnetic data is an emerging technique in obtaining subsurface density and magnetization source distributions. However, the absence of geophysical constraints, inflexibility of structural coupling and oversimplified features of synthetic data restrict the data-driven deep learning joint inversion, outputting models inconsistent with geophysical observations and geological priors. We propose a physics-informed deep learning framework for joint inversion of gravity and magnetic data. The data-driven pre-training is initially utilized by conducting end-to-end supervised training, learning the synthetic features from training dataset. With inverted density and magnetization distributions using pre-trained network, the data misfit and structural losses are calculated for physics-informed fine-tuning of the network. The embedment of physics-informed fine-tuning optimizes data-driven pre-trained network while retaining swift model reconstruction ability, generating models with improved data fitting and model reconstruction of the consistent source regions. The proposed framework is tested on two sets of synthetic examples with different structural homologies and applied to the field data of the Jining iron deposit (northern China). The joint inversion generates density and magnetization distributions for hematite and magnetite and indicates the possibile presence of a regional magnetic basement caused by the high-susceptibility amphibole magnetite quartzite in the Taishan Group. The proposed physics-informed deep learning framework for joint inversion demonstrates the potential of integrating multiple geophysical data and enhances the geophysical consistency in geological modeling.

How to cite: Yan, X., Liu, S., and Lv, M.: A Deep Learning Framework for Joint Inversion of Gravity and Magnetic Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12390, https://doi.org/10.5194/egusphere-egu26-12390, 2026.

EGU26-12493 | ECS | Orals | EMRP2.2

Validation of Drone-Borne Aeromagnetic Surveys Using Multi-Altitude Measurements in Rugged Terrains, Taiwan 

Chung-Wei Chang, Wen-Jeng Huang, Chien-Chih Chen, and Jui-Yu Kao

Geothermal energy is an essential renewable resource whose effective development relies on subsurface structure, particularly in regions with high geothermal potential. Magnetic surveying serves as a fundamental geophysical tool in this context, enabling the identification of concealed intrusions, estimation of source depths, and delineation of buried dykes or faults. While regional airborne campaigns offer efficient coverage, their resolution is often limited by wide survey-line spacing and high flight altitudes. Conversely, ground-based surveys, though detailed, are frequently hindered by rugged terrain and accessibility issues. Drone-borne aeromagnetic surveys address these limitations, providing high-resolution datasets in areas with complex topography.

In this study, we utilized a total-field scalar magnetometer integrated with a multicopter Unmanned Aerial System (UAS) to acquire magnetic measurements. The UAS followed pre-programmed survey lines defined by GPS waypoints and employed terrain-following flight modes at constant altitudes no higher than 120 m above ground level, which are substantially lower than those of conventional airborne surveys and allow measurements to be acquired closer to subsurface magnetic sources. Surveys were conducted at multiple altitudes to calculate vertical magnetic gradients, which serve as essential constraints for modeling subsurface magnetic susceptibility distributions. The data processing workflow comprised spike removal, International Geomagnetic Reference Field (IGRF) correction, and diurnal correction. The processed data were subsequently gridded using the natural neighbor interpolation method to generate magnetic anomaly maps.

Our drone-borne aeromagnetic surveys in volcanic regions have demonstrated strong consistency with existing aeromagnetic datasets while offering significantly enhanced spatial density. This study extends the application of drone-borne aeromagnetic surveying to a metamorphic formation with lava flows. Distinct magnetic anomaly patterns are observed at different flight altitudes. Ongoing research involves the application of computational methods and modeling to analyze these altitude-dependent phenomena and refine the interpretation of subsurface magnetic source distributions.

How to cite: Chang, C.-W., Huang, W.-J., Chen, C.-C., and Kao, J.-Y.: Validation of Drone-Borne Aeromagnetic Surveys Using Multi-Altitude Measurements in Rugged Terrains, Taiwan, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12493, https://doi.org/10.5194/egusphere-egu26-12493, 2026.

Gravity‐Derived Moho Depth of Egypt: Insights from Lithospheric-Scale Gravity Inversion and Comparison with Global Crustal Models

Mohammad Shehata1,2, Hakim Saibi1

1Geosciences Department, College of Science, United Arab Emirates University, 15551, Al-Ain, United Arab Emirates

2Department of Geology, Faculty of Science, Port Said University, Port Said 42522, Egypt

 

Reliable constraints on Moho depth are fundamental for understanding lithospheric structure and tectonic evolution, yet estimates across Egypt and northeastern Africa remain uneven in coverage and resolution. Seismic constraints are restricted to discrete locations, while global crustal models mainly capture long-wavelength features and may not resolve crustal thickness contrasts across different tectonic domains. Here we present a country-scale Moho depth model for Egypt derived from GOCE satellite gravity, providing continuous regional coverage for evaluating tectonically controlled crustal thickness variations.

Bouguer gravity anomalies were computed from GOCE satellite gravity data, complemented where appropriate by terrestrial observations, and corrected for topography, bathymetry, and sedimentary cover. Moho geometry was estimated using frequency-domain Parker–Oldenburg iterative inversion incorporating laterally variable crust–mantle density contrasts derived from the CRUST1.0 model, allowing spatial variations in crustal composition and thickness to be explicitly accounted for (Shehata and Mizunaga, 2022). The resulting Moho model reveals systematic crustal thickness variations that closely correspond to Egypt’s tectonic architecture, with shallow Moho depths (~18–22 km) beneath extensional domains associated with Red Sea rifting, intermediate depths (~28–34 km) in transitional zones such as the Nile Delta and Sinai, and thick crust (>40–43 km) across the Western Desert and southern Egypt. Sharp lateral Moho gradients delineate boundaries between these regimes, indicating localized strain accommodation during rift development. Comparison with CRUST1.0 (Laske et al., 2013), GEMMA (Reguzzoni et al., 2013), and the seismic-based Moho compilation of Tugume et al., 2013) shows overall agreement at long wavelengths, while localized deviations occur in rifted and transitional regions due to differences in data resolution and methodological sensitivity. These results demonstrate that tectonic regime exerts a first-order control on Moho depth beneath Egypt and highlight the value of GOCE-based gravity inversion for improving lithospheric characterization in regions of limited seismic coverage.

References

Laske, G., Masters, G., Ma, Z., Pasyanos, M., 2013. Update on CRUST1. 0—A 1-degree global model of Earth’s crust, in: Geophysical Research Abstracts. p. 2658.

Reguzzoni, M., Sampietro, D., Sansò, F., 2013. Global Moho from the combination of the CRUST2. 0 model and GOCE data. Geophys. J. Int. 195, 222–237.

Shehata, M.A., Mizunaga, H., 2022. Moho depth and tectonic implications of the western United States: insights from gravity data interpretation. Geosci. Lett. 9, 23.

Tugume, F., Nyblade, A.A., Julia, J., Van der Meijde, M., 2013. Crustal shear wave velocity structure and thickness for Archean and Proterozoic terranes in Africa and Arabia from modeling receiver functions, surface wave dispersion, and satellite gravity data. Tectonophysics 609, 250–266.

How to cite: Shehata, M. and Saibi, H.: Gravity‐Derived Moho Depth of Egypt: Insights from Lithospheric-Scale Gravity Inversion and Comparison with Global Crustal Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12524, https://doi.org/10.5194/egusphere-egu26-12524, 2026.

EGU26-13520 | Posters on site | EMRP2.2

A Compartmentalized Elevation Model Approach to Terrain Correction in Microgravity Surveys 

Sohail Shahzad and Khan Zaib Jadoon

Microgravity surveying is a high-resolution geophysical technique widely used for detecting subsurface voids, karst features, and localized density variations in engineering, environmental, and geological investigations. However, in complex environments such as steep mountainous terrain, narrow valleys, and urban or built-up areas, standard terrain correction approaches often fail to adequately account for fine-scale topographic variations and man-made structures. These limitations can introduce significant distortions in Bouguer anomalies, particularly at the microGal sensitivity level required for microgravity applications.

This research presents an enhanced terrain correction methodology specifically tailored for microgravity surveys conducted in complex natural and artificial environments. The proposed approach integrates high-resolution elevation data derived from Digital Terrain Models (DTMs), conventional topographic surveys, and 3D LiDAR datasets to construct detailed compartmentalized mass models around each gravity observation point. Surrounding terrain and structures are discretized into three-dimensional volumetric compartments characterized by spatial position, elevation, size, and density. Unlike conventional methods, the approach allows the assignment of variable densities to individual compartments, enabling accurate representation of heterogeneous materials such as rock, air-filled voids, buildings, and structural components.

Gravitational acceleration contributed by each compartment is calculated using Newtonian gravity principles, and the vertical component relevant to terrain correction is extracted and summed to compute station-specific corrections. The methodology is implemented using a database-driven computational framework to efficiently handle the large number of calculations involved. Results demonstrate that the proposed technique significantly improves terrain correction accuracy, effectively capturing the gravitational influence of steep slopes, narrow valleys, and complex urban infrastructure. The integration of 3D LiDAR-derived models enhances spatial resolution and supports microGal-level precision. The proposed compartmentalized terrain correction approach provides a scalable, automated, and accurate alternative to traditional methods, offering substantial benefits for microgravity investigations in rugged terrain and densely built environments.

How to cite: Shahzad, S. and Jadoon, K. Z.: A Compartmentalized Elevation Model Approach to Terrain Correction in Microgravity Surveys, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13520, https://doi.org/10.5194/egusphere-egu26-13520, 2026.

EGU26-15624 | ECS | Orals | EMRP2.2

Airborne Vector Gravimetry Method Based on Independent Gyros Observations 

Wenkai Xiang, Shaokun Cai, Yan Guo, Juliang Cao, Zhiming Xiong, Kaixin Luo, Ruihang Yu, and Meiping Wu

In airborne vector gravimetry algorithms based on SINS/GNSS integrated navigation, the ultimate accuracy of horizontal attitude resolution is primarily constrained by the combined effects of horizontal gravity disturbances and accelerometer measurement errors. Gravity disturbances along the survey line enter the error propagation equations of the strapdown inertial navigation system (SINS) via the sensitivity of accelerometers, forming a closed-loop coupled error propagation chain related to horizontal gravity disturbances. This increases the difficulty of error processing and gravity vector determination. To address this issue, this paper proposes an airborne vector gravimetry method based on independent gyroscopic observation. The method introduces an independent gyros-based attitude determination approach into the traditional SINS/GNSS integrated navigation algorithm. It utilizes the gyroscope assembly of the SINS to independently update the attitude in the inertial frame. The geographic position and time information from GNSS are then used to transform this inertial-frame attitude to the navigation frame for use. A key feature of this method is that it does not employ accelerometer measurements during the attitude update process, thereby avoiding the influence of accelerometer errors and gravity disturbances on the horizontal attitude and achieving decoupling of the closed-loop error propagation chain. Building upon this foundation, the study investigates the linear mapping relationship between the horizontal attitude errors independently resolved by the gyroscope and the horizontal gravity disturbances. Error compensation for airborne gravity vector measurements is performed using gravity anomaly information derived from the EGM2008 model, with both simulated and field data employed for validation. The airborne gravity survey experiments demonstrate that the internal consistency accuracies for the eastward, northward, and upward gravity anomaly components are 1.53 mGal, 2.34 mGal, and 0.59 mGal, respectively, with a spatial resolution of approximately 3 km. This method significantly enhances the decoupling capability between accelerometer measurement errors and gravity disturbances, thereby improving the measurement accuracy of horizontal gravity components.

How to cite: Xiang, W., Cai, S., Guo, Y., Cao, J., Xiong, Z., Luo, K., Yu, R., and Wu, M.: Airborne Vector Gravimetry Method Based on Independent Gyros Observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15624, https://doi.org/10.5194/egusphere-egu26-15624, 2026.

EGU26-15998 | ECS | Orals | EMRP2.2

Hex-OSGM: Incremental Gravity Field Learning on Adaptive Hexagonal Meshes for Robust Passive Navigation 

Renjie Zhao, Ruihang Yu, Kaixin Luo, Zhiming Xiong, Juliang Cao, Shaokun Cai, Yan Guo, and Meiping Wu

    Gravity-matching navigation—a self-contained and passive navigation modality—depends critically on the accuracy and resolution of the background gravity field and the adaptability of the matching algorithm,Current gravity modeling methods, however, are limited by slow model updates and inefficient storage under dynamic operating conditions. To overcome these challenges, we introduce a novel gravity-matching framework that integrates incremental learning with adaptive mesh optimization.

    Our approach proceeds in three key stages. First, a global gravity field is rapidly initialized using a spherical-harmonics model trained via an Extreme Learning Machine (ELM). We then employ an online sequential ELM (OS-ELM) to incrementally assimilate posterior gravity information—whether obtained in real time or fused from multi-source observations—thereby enabling timely model updates and continuous refinement of field fidelity.

    Second, we systematically evaluate the sensitivity of batch-matching algorithms (e.g., ICCP and contour matching) to interpolation density and derive an adaptive density-selection criterion that incorporates prior map information content, vehicle velocity, and inertial navigation system error growth. To improve storage and computational efficiency, we replace conventional rectilinear grids with a hexagonal tessellation for field discretization. Theoretical analysis and experimental results confirm that, at equal nominal resolution, the hexagonal lattice reduces both model and localization errors while its structural isotropy enhances the stability and convergence of batch matching across diverse heading angles.

    Third, we introduce an encrypted interpolation strategy centered on hexagonal cell centroids. This approach increases effective resolution with only a minor increase in storage, thereby improving the algorithm’s ability to resolve subtle gravity features. Numerical simulations and field data demonstrate that the proposed framework sustains high-precision matching performance while significantly reducing storage and computational burdens, offering a promising technical pathway toward long-endurance, robust gravity-matching navigation in complex environments.

How to cite: Zhao, R., Yu, R., Luo, K., Xiong, Z., Cao, J., Cai, S., Guo, Y., and Wu, M.: Hex-OSGM: Incremental Gravity Field Learning on Adaptive Hexagonal Meshes for Robust Passive Navigation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15998, https://doi.org/10.5194/egusphere-egu26-15998, 2026.

EGU26-18750 | ECS | Posters on site | EMRP2.2

An Inversion Method for Moho Depth Distribution Characteristics in the Bohai Sea and Its Adjacent Areas Based on the Improved Bott-Parker Method 

Guanghong Lan, Juliang Cao, Zhiming Xiong, Kaixin Luo, Ruihang Yu, Shaokun Cai, Yan Guo, and Meiping Wu

Abstract. The Bohai Sea and its adjacent areas (116.5°~123.5°E, 36.5°~41.5°N) are located in eastern China, serving as a critical marine-continental transition zone in the eastern part of the country. Acquiring high-precision distribution characteristics of the Moho depth in this region is of great significance for understanding the local deep tectonic features and the distribution of mineral resources such as oil and gas. Owing to the high cost of seismic surveys, it is difficult to obtain the overall Moho topography of the region. Therefore, based on the latest generation of SWOT-03 satellite gravity data, this study uses the improved Bott-Parker method to invert a high-resolution Moho topography with a resolution of 1′×1′ in the Bohai Sea and its adjacent areas. First, Bouguer correction was applied to the SWOT-03 free-air gravity anomalies to derive the Bouguer gravity anomalies of the study area. To separate the Moho gravity anomalies, which reflect the distribution characteristics of the Moho depth, from the Bouguer gravity anomalies, an 8th-order wavelet multiscale decomposition was performed on the Bouguer gravity anomalies, generating the corresponding wavelet approximations and wavelet details. Then, the average radial logarithmic power spectrum analysis method was used to calculate the approximate source depths of the wavelet details of each order, thus obtaining the gravity anomalies that represent Moho undulation. Finally, the improved Bott-Parker method was employed to invert the high-resolution Moho topography of the Bohai Sea and its adjacent areas. Specifically, the improved Bott-Parker method obtains the initial Moho topography via linear regression using known seismic Moho data and Moho gravity anomalies derived from wavelet multiscale decomposition, and then continuously corrects the Moho topography using the gravity difference between the forward-calculated values from the Parker method and the observed gravity values. Compared with the traditional Parker-Oldenburg method, the improved Bott-Parker method avoids the need to set the cutoff frequency of the filter. The results demonstrate that the average Moho depth in the Bohai Sea and its adjacent areas is 32.98 km, with a variation range of 24.26~57.22 km, and multiple Moho uplift and depression zones are present in the region. The inverted Moho topography is basically consistent with the Crust1.0 global crustal model, which can well reflect the distribution characteristics of the Moho depth in the Bohai Sea and its adjacent areas as a whole. This study has certain guiding significance for understanding the regional tectonic features and conducting oil and gas exploration.

Keywords: SWOT-03 satellite gravity data; Moho depth; Gravity inversion; Wavelet multi-scale decomposition;Improved Bott-Parker method

How to cite: Lan, G., Cao, J., Xiong, Z., Luo, K., Yu, R., Cai, S., Guo, Y., and Wu, M.: An Inversion Method for Moho Depth Distribution Characteristics in the Bohai Sea and Its Adjacent Areas Based on the Improved Bott-Parker Method, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18750, https://doi.org/10.5194/egusphere-egu26-18750, 2026.

EGU26-19348 | Posters on site | EMRP2.2

Aeromagnetic Mapping in the Northern Tihamah region, Western Yemen 

Marwan Al-Badani and Fausto Ferraccioli

The basement geology of Yemen is related to the evolution of the late Archean to late Neoproterozoic Arabian-Nubian Shield and contains key records of microplate and island arc accretion during Gondwana assembly. Furthermore, Yemen also preserves important igneous and structural records related to the multi-stage extension and opening of the Gulf of Aden-Red Sea Rift System.

Here we focus on the interpretation of aeromagnetic anomaly data in western Yemen by analysing part of a magnetic anomaly compilation for the whole of Yemen that includes data collected from 26 different airborne surveys flown between 1976 and 1985.

Our reduced to the pole map reveals magnetic anomalies of varying amplitudes and wavelengths, reflecting differences in lithology, structure, and source depth. We applied edge-detection techniques, including tilt angle derivative, total horizontal derivative of the tilt angle, and 3D Euler deconvolution to aid depth to source estimation.

An intriguing result is the newly defined extent of largely buried Cenozoic igneous intrusions that we image from the scant exposures along the southern uplifted rift-related great escarpment to the downthrown block in the northern Tihamah plain. The trend of these anomalies lies at relatively high angle to the rift flank escarpment but is co-linear with some of the trends imaged in the Precambrian basement, suggesting an important role of the inherited structures on much later magma emplacement. To further contextualise our regional results we combine the data from western Yemen with lower resolution publically available data from adjacent sectors of the Arabian shield and the Red Sea Rift and discuss some of the potential tectonic implications.

How to cite: Al-Badani, M. and Ferraccioli, F.: Aeromagnetic Mapping in the Northern Tihamah region, Western Yemen, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19348, https://doi.org/10.5194/egusphere-egu26-19348, 2026.

EGU26-19968 | Posters on site | EMRP2.2

A Multi-Method Gravity Workflow for Reliable Structural Mapping in Northern Tunisia 

imen hamdi, Mohamed Sobh, Adnen Amiri, and inoubli Mohamed hédi

High-resolution gravity data were used to assess their potential and limitations as a subsurface investigation tool to constrain key geological structures and support georesource exploration in Northwestern Tunisia. In this structurally complex area, methodological choices—particularly those related to regional–residual separation, derivative filtering, interpolation schemes, and Euler-based depth-estimation parameters—significantly influence the geometry, continuity, and uncertainty of interpreted lineaments.

To mitigate these effects, we applied an integrated multi-stage workflow combining residual anomaly mapping, derivative filters, tilt-angle transformation, power-spectrum analysis, Euler deconvolution of horizontal gradients (EHD), and 3D Euler solutions. These complementary approaches delineate subsurface fault systems and highlight deep structural controls on Triassic salt diapirs and associated Pb–Zn mineralization. The results reveal a dominant NE–SW structural corridor with fault depths reaching ~1.75 km, spatially correlating with known mineralized sites and salt-dome boundaries.

To further enhance structural reliability and quantify subsurface density distributions, the workflow incorporates 3D gravity inversion. The inversion model helps image density contrasts associated with the Triassic evaporites, validating interpreted lineaments and refining depth estimates derived from derivative-based and Euler approaches. Integrating forward–inverse modelling with classical interpretation tools not only enhances the structural understanding but also provides a clear workflow, helping users assess the reliability and limitations of gravity-derived structural maps in tectonic complex areas.

 

How to cite: hamdi, I., Sobh, M., Amiri, A., and Mohamed hédi, I.: A Multi-Method Gravity Workflow for Reliable Structural Mapping in Northern Tunisia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19968, https://doi.org/10.5194/egusphere-egu26-19968, 2026.

EGU26-21409 | Orals | EMRP2.2

Enhanced magnetic and gravity imaging of the crustal basement beneath the northern Wilkes Subglacial Basin in East Antarctica 

Fausto Ferraccioli, Shi Quan Ooi, Marwan A. Al-Badani, Duncan Young, Donald Blankenship, Egidio Armadillo, Joerg Ebbing, and Martin Siegert

The Wilkes Subglacial Basin (WSB) is one of the largest tectonic features in East Antarctica as it stretches for almost 1600 km from the Southern Ocean towards South Pole. Significant research has focussed on the tectonic origin of the basin with competing models ranging from Paleozoic, Mesozoic and Cenozoic extensional models to flexural models related to the Cenozoic uplift of the Transantarctic Mountains. Comparatively little effort has however been placed on investigating the cryptic basement of the WSB despite its key location at the transition between the exposures of the Archean-Mesoproterozoic Terre Adelie Craton and the late Neoproterozoic to Ordovician age Ross Orogen.

Here we present enhanced aeromagnetic and airborne gravity imaging augmented by satellite magnetic and satellite gravity data and comparisons with formerly adjacent southeastern Australia to redefine key features of the basement in the northern WSB region.

We show that a prominent magnetic low located beneath the Western Basins within the WSB is not caused by a ca 3 km thick Cambrian rift basin as previously proposed (Ferraccioli et al., 2009, Tectonophysics) but images instead a linear Archean crustal ribbon extending further north to exposures of Archean rocks in the Terre Adelie craton and in the Gawler Craton. Cambrian sedimentary basins are confirmed further east beneath the northern Central Basins. Prominent magnetic highs along the eastern flank of the WSB and at the edge of the southern Central Basins were previously interpreted to reveal Ross age igneous basement associated with an arc-back arc system. However, the occurrence of longer wavelength satellite magnetic anomalies both in the WSB and at the edge of the Gawler Craton and in the Curnamona Craton in Australia lead us to propose an alternative hypothesis that predicts the occurrence of more extensive Paleo to Mesoproterozoic basement than previously inferred. Furthermore, a prominent linear residual gravity anomaly along the western flank of the WSB is interpreted here as reflecting uplifted mafic lower crust associated with Paleoproterozoic rifting. High amplitude aeromagnetic anomalies may reflect coeval banded iron formations associated at shallower crustal levels with such Paleoproterozoic rifting processes.

By comparing gravity signatures over the WSB and southern Australia and by incorporating recent seismic constraints at the transition between the Gawler Craton and the Delamerian Orogen we reassess the extent and architecture of both the Precambrian and Cambrian basement.

Overall, our results and models have significant implications for tectonic studies of the basement of the WSB, including better defining the role of inherited tectonics structures on the more recent  Paleozoic, Mesozoic to Cenozoic evolution of the WSB. Furthermore, the larger degree of heterogeneity in the crustal basement identified here will help inform next generation models of intracrustal contributions to geothermal heat flow  beneath this key sector of the East Antarctic Ice Sheet.

How to cite: Ferraccioli, F., Ooi, S. Q., Al-Badani, M. A., Young, D., Blankenship, D., Armadillo, E., Ebbing, J., and Siegert, M.: Enhanced magnetic and gravity imaging of the crustal basement beneath the northern Wilkes Subglacial Basin in East Antarctica, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21409, https://doi.org/10.5194/egusphere-egu26-21409, 2026.

EGU26-21850 | Posters on site | EMRP2.2

Quantitative Assessment of CO2 Leakage Using Time-Lapse Gravity Inversion 

Maurizio Milano, Alessia Ianniello, Marco Maiolino, Luigi Bianco, and Maurizio Fedi

We propose an innovative approach for the interpretation of time-lapse gravity data aimed at estimating subsurface mass variations associated with CO2 injection and storage. The method is based on the Extremely Compact Source (ECS) inversion technique (Maiolino et al., 2024), which is used to isolate the individual contributions of discrete CO2 mass accumulations in the subsurface and to quantify their associated excess mass.

To date, ECS inversion has been primarily applied as a filtering strategy to remove regional-scale contributions from potential field data or to separate the effects of closely spaced sources. The approach relies on an iterative inversion of potential field observations to derive a subsurface model composed of source distributions with minimal volumetric extent, referred to as atoms, simultaneously ensuring a low data misfit. A key advantage of the method is that it does not require any a priori information about subsurface properties.

Once the ECS model is obtained, the excess mass associated with each source contributing to the observed gravity anomaly can be readily computed. In this study, we demonstrate that the proposed approach enables precise identification of CO2 accumulations within the reservoir and allows for accurate estimation of net mass variations related to both stored CO2 and leakage occurring along permeable fault zones.

 

How to cite: Milano, M., Ianniello, A., Maiolino, M., Bianco, L., and Fedi, M.: Quantitative Assessment of CO2 Leakage Using Time-Lapse Gravity Inversion, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21850, https://doi.org/10.5194/egusphere-egu26-21850, 2026.

EGU26-396 | ECS | Posters on site | EMRP2.3

The Potential of Radiomagnetotellurics for Detecting Dike Instabilities 

Ramon Vanoli, Dieter Werthmüller, Ute Weckmann, and Paula Rulff

With rising sea levels and frequent heavy rainfall, water retention structures such as dikes become increasingly susceptible to failure. Therefore, there is a need to monitor such structures in a time and cost-efficient manner, and sufficient resolution. Electromagnetic geophysics could potentially be used for this purpose, since instability features such as water underflow or animal paths change the electrical conductivity inside the dike. In this project, we study if the Radiomagnetotelluric method can be used to investigate dikes for instability features.  First, we perform forward and inverse simulations with a synthetic dike model to verify the feasibility of the method for the purpose of detecting dike instabilities. Next, we will define suitable frequencies and measurement setups through a synthetic survey design study. Subsequently, we will apply the newly acquired knowledge from the synthetic experiments to conduct a Radiomagnetotelluric survey on a dike in the Netherlands. Dikes are often situated in populated areas, which means that significant cultural noise must be accounted for during the data processing. Through 2D and 3D inversions we will generate resistivity models of the Radiomagnetotelluric data and compare them to a resistivity model obtained from ERT data to validate the results. The final objective is to evaluate the potential of the method for practical dike monitoring and give recommendations for its implementation.

How to cite: Vanoli, R., Werthmüller, D., Weckmann, U., and Rulff, P.: The Potential of Radiomagnetotellurics for Detecting Dike Instabilities, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-396, https://doi.org/10.5194/egusphere-egu26-396, 2026.

The North China Craton (NCC), the largest and oldest craton in China, has experienced multiple significant crustal growth and evolutionary events. Its northern margin adjoins the Central Asian Orogenic Belt (CAOB), forming a complex tectonic transition zone. During the Late Permian to Triassic period, the subduction and subsequent closure of the Paleo-Asian Ocean led to the formation of the CAOB, a process widely believed to have altered the composition and properties of the lithospheric mantle at the northern margin of the NCC. This study aims to use the Magnetotelluric (MT) method to investigate the impact of the subduction and accretion of the Paleo-Asian Ocean on the northern margin of the NCC and to explore the global significance of continental reworking as a deep carbon cycling mechanism.

We utilized long-period MT data from the SinoProbe NCC MT array and two MT profiles from the CAOB, totaling 114 MT stations. After data processing and analysis, we performed 3D inversions using the ModEM package. We found that the lithospheric mantle of the Yinshan-Yanshan orogenic belt in the northern NCC mainly exhibits low resistivity, and a large-scale conductor exists from the lower crust to the upper mantle in the central and northern parts of the Ordos Block, indicating that the mantle may have undergone some degree of modification. These may be related to the collision-accretionary orogenesis of the CAOB, the sulfur- and carbon-bearing sediments brought in by the subduction plate separated from the sinking plate at depth to form sedimentary diapires. In this process, carbonate melting and carbon precipitation may have occurred.

These findings indicate that the crust at the northern margin of the NCC has experienced tectonic reactivation, with the stretching and extension of the lower crust facilitating the migration and mixing of deep melts. This process likely involved crust-mantle interaction, leading to partial modification of the composition of the ancient crustal basement. The complexity of crustal composition and structure within the CAOB reflects the characteristics of the young crust of the Phanerozoic accretionary orogenic belt. We believe that these electrical characteristics are all related to the deep carbon cycling processes induced by the subduction, accretion of the Paleo-Asian Ocean, and the reworking of the NCC continent, providing important constraints on the deep physical properties for understanding the compositional evolution mechanisms and characteristics of continental crust at different stages of growth.

 

*This research is funded by Deep Earth Probe and Mineral Resources Exploration - National Science and Technology Major Project (2024ZD1000100-06-04) and NSFC (42074089).

How to cite: Li, Y., Zhang, L., Jin, S., Becken, M., Wei, W., and Ye, G.: The Role of the Closure of the Paleo-Asian Ocean in Lithospheric Modification of the Western North China Craton: implications from magnetotelluric array data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-752, https://doi.org/10.5194/egusphere-egu26-752, 2026.

EGU26-785 | ECS | Posters on site | EMRP2.3

Surface-to-borehole Controlled-source Electromagnetics for monitoring temperature changes in a geothermal aquifer 

Suzanne van Noordt, Guy Drijkoningen, Alexandros Daniilidis, and Paula Rulff

A High Temperature Aquifer Thermal Energy Storage system will be installed on the TU Delft campus, The Netherlands, utilising an aquifer at 120-180 m depth to store hot water (>60 °C). For optimal recovery efficiency, it is essential that the injected water stays near the injector well until it can be extracted, and that there is no mixing with cold water. By monitoring the spread of injected water using Controlled-Source Electromagnetics, the heat transport in this subsurface storage system could be better understood. For this, a  surface-to-borehole survey design was proposed, sensitive to the resistivity at the depth of the aquifer through the vertical component of the electric field. 3D time-lapse data will be acquired using receivers inside a monitoring borehole and horizontal electric dipole sources surrounding the site. Optimal source positions will be determined through a feasibility study, using forward-modelling and inversion of synthetic data. By relating the resistivity of the water to its temperature, this data can be used to image hot plume propagation over time. However, the relationship between conductivity and temperature is expected to vary between sites and for large temperature ranges. Laboratory measurements will therefore be performed, uncovering site-specific resistivity-temperature relationships to improve the interpretation of Controlled-Source Electromagnetic data. Lastly, a future research interest lies in the combination of monitoring data with thermodynamic modelling. Through workflows of data-assimilation or process-based inversion, these methods could complement each other, leading to an enhanced understanding of heat flow in the aquifer.

How to cite: van Noordt, S., Drijkoningen, G., Daniilidis, A., and Rulff, P.: Surface-to-borehole Controlled-source Electromagnetics for monitoring temperature changes in a geothermal aquifer, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-785, https://doi.org/10.5194/egusphere-egu26-785, 2026.

Identifying geomagnetic pulsations is crucial for monitoring and issuing early warnings of space weather hazards that threaten modern technological infrastructure. This study examines the relationship between variations in magnetotelluric data quality and geomagnetic disturbances, aiming to develop an early space weather warning system utilizing existing magnetotelluric station networks. Magnetotelluric surveys measure natural electromagnetic signals to study subsurface structures, but signal quality in the 0.1–10 Hz frequency range—known as the dead band—is typically poor during geomagnetically quiet periods due to weak source fields. Geomagnetic disturbances significantly enhance signal strength in this band, markedly improving measurement quality. We developed a parameter called the linearity ratio, based on electromagnetic field linearity, to automatically detect geomagnetic disturbances. Additional metrics including phase differences and energy are used to comprehensively monitor data quality changes. Compared to traditional methods, this approach requires minimal computational resources, enables real-time monitoring, directly utilizes existing magnetotelluric infrastructure, and provides physically meaningful indicators. Analysis of two representative events using data from the Memambetsu station in Japan demonstrates that this method reliably identifies geomagnetic activity with minute-scale temporal resolution. Geomagnetic storms comprise initial, main, and recovery phases, with the main phase posing the greatest threat to critical infrastructure. Our approach complements existing geomagnetic storm forecasts by detecting the initial phase, providing early warning before the most hazardous conditions develop. This offers a cost-effective space weather monitoring solution by repurposing established ground-based electromagnetic observation networks.

How to cite: Chen, H.: Identifying Pc2 Geomagnetic  Pulsation through Magnetotelluric Data Quality Analysis in Dead Band Frequencies, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1474, https://doi.org/10.5194/egusphere-egu26-1474, 2026.

EGU26-1578 | Orals | EMRP2.3 | Highlight

The power of modularity in open-source projects 

Dieter Werthmüller, Seogi Kang, Thomas Günther, Wouter Deleersnyder, María Carrizo Mascarell, and Lukas Aigner

The advantages of well-documented and modularly designed open-source projects starts to shine when they allow for the combination of different tools to create new possibilities. We have achieved this in the last few years within the electromagnetic (EM) geophysics community.

PyGIMLi is an open-source library for multi-method modelling and inversion in geophysics. It is particularly strong in electrical resistivity tomography, induced polarization, magnetics, and seismic refraction tomography, as well as in joint inversions.

SimPEG is an open-source Python package for simulation and gradient-based parameter estimation in geophysical applications. It provides strong capabilities, particularly for modelling gravity, magnetics, direct current resistivity, induced polarization, and frequency- and time-domain electromagnetic data. Additionally, it provides a joint inversion capability. However, the analytical 1D forward modelling is, currently, limited to loop-loop configurations. Furthermore, for 3D EM modelling, it uses a direct solver with a large memory requirement.

The emsig project contains a variety of codes. One of them is empymod, a semi-analytical electromagnetic code for layered media that can model any source-receiver configuration. Another one is emg3d, a three-dimensional modeller for EM diffusion. It provides a matrix-free multigrid solver, which means that it has a comparatively low memory footprint. However, both of these codes are purely forward modelling codes, and contain no possibility for inversions.

We will present how these codes can be combined to use the forward modelling capabilities of emsig, together with the inversion capabilities of SimPEG and pyGIMli. This not only elevates all codes to create new tools in the form of SimPEG(emsig) and pyGIMLi(emsig), but more importantly, it also allows for comparisons between different frameworks. While doing these exercises, we did encounter some struggles and concepts that need to be modularized better and be improved in the future. In particular, forward modelling codes should provide easy ways to obtain the forward response as well as the (adjoint-state or analytical) gradient. Inversion codes, on the other hand, should be able to run the inversion without knowledge of the survey configuration or any of the underlying method, just with the forward responses and the gradients. These are ideas that are often not thought of when starting a new project, but they would make life much easier if they were, which is why we offer guidelines for developers to improve the modularity of future forward modeling and inversion codes.

How to cite: Werthmüller, D., Kang, S., Günther, T., Deleersnyder, W., Carrizo Mascarell, M., and Aigner, L.: The power of modularity in open-source projects, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1578, https://doi.org/10.5194/egusphere-egu26-1578, 2026.

Low-frequency electromagnetic sounding, particularly magnetotellurics (MT) and audio-magnetotellurics (AMT), is widely applied to characterize subsurface resistivity. In operational settings, however, impedance estimation is frequently constrained by cultural noise, power-line harmonics, grounding artifacts, and instrument drift, which can substantially degrade data reliability. Under such conditions, automated selection of usable time windows and principled weighting of frequency bands become critical determinants of estimation stability. This literature review examines methodological approaches to window selection and frequency-band weighting in MT/AMT processing, focusing on coherence- and stability-based quality metrics and decision rules that span hard rejection and soft weighting. The review also discusses how these quality control procedures interact with transfer-function estimation workflows and reporting practices. Emphasis is placed on reproducibility and the transparent specification of quality control criteria, while summarizing commonly reported applicability conditions, limitations, and failure modes in the existing literature.

How to cite: Liu, C.-Y.: Automated Window Selection and Frequency-Band Weighting for Reliable Magnetotelluric and Audio-Magnetotelluric Impedance Estimation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2095, https://doi.org/10.5194/egusphere-egu26-2095, 2026.

EGU26-2811 | ECS | Posters on site | EMRP2.3

Prospecting Deep Targets Potentially Mineralized with Copper South of the Seival Mines, Camaquã Basin, Southern Brazil 

Marina Barros, Cesar Moreira, Henri Masquelin, Lenon Ilha, Sissa Kumaira, and Daniela Kuranaka

The Seival Mines comprise a group of open-pit copper mines that have been inactive for more than 60 years, located in the municipality of Caçapava do Sul, southern Brazil. In the region, volcanic, subvolcanic, and volcaniclastic rocks of the Hilário Formation crop out; this formation belongs to the Bom Jardim Group, a unit of the Camaquã Basin (450–620 Ma). The Seival area hosts hydrothermal copper sulfide deposits within volcanic rocks of shoshonitic affinity, emplaced in brittle zones controlled by structures with predominant N–NE and NW trends. Enrichment in Cu, Au, and Ag within andesitic dikes suggests that intrusions acted as important conduits for the hydrothermal processes responsible for metallogenesis. Despite Brazil’s high potential for the discovery of new mineral deposits, mineral exploration faces increasing challenges related to the growing scarcity of economically viable outcropping deposits. This context justifies the development of more detailed geological and geophysical studies, combined with the adoption of new strategies and subsurface investigation technologies. In this study, the Transient Electromagnetic (TEM) geophysical method was applied using the WALKTEM 2 system (ABEM). Surveys were carried out in a centre-loop configuration, with a 100 × 100 m transmitter loop and an RC-200 receiver antenna (10 × 10 m), operating in dual-moment mode. Three data profiles were acquired in the study area, totaling 14 electromagnetic soundings spaced at 250 m intervals. Data processing and inversion were performed using the SPIA and Workbench software packages. The resulting electrical resistivity sections reveal significant lateral and vertical variations, with resistivity values ranging approximately from 10 to 2000 Ω·m. In general, an upper unit is characterized by resistivity values exceeding 1000 Ω·m, associated with volcanic rocks of the Hilário Formation, whose thickness varies along the profiles. At depths of around 400 m, subhorizontal layers with resistivity values below 60 Ω·m and thicknesses of up to 200 m are observed. This horizon is possibly related to sandstones and conglomerates of the Maricá Group, the basal unit of the Camaquã Basin. The low-resistivity layer at this interface is a clear indication of the presence of conductive materials, which in the regional context are represented by sulfides hosted within a porous interface during the ascent of hydrothermal fluids responsible for the genesis of the Seival deposits. The identification of this potentially mineralized interface highlights the regional potential for deep copper deposits, based on a relatively rapid and versatile geophysical diagnosis.

Keywords: copper, mineral deposit, transient electromagnetics, resistivity

How to cite: Barros, M., Moreira, C., Masquelin, H., Ilha, L., Kumaira, S., and Kuranaka, D.: Prospecting Deep Targets Potentially Mineralized with Copper South of the Seival Mines, Camaquã Basin, Southern Brazil, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2811, https://doi.org/10.5194/egusphere-egu26-2811, 2026.

EGU26-4367 | Orals | EMRP2.3

Building uncertainty-aware subsurface models with 3D magnetotelluric inversion 

Pankaj K Mishra, Jochen Kamm, Cedric Patzer, Uula Autio, and Mrinal K Sen

Magnetotellurics (MT) images electrical conductivity, a property influenced by fluids, alteration, graphite, and partial melt. Because many different subsurface configurations can explain the MT responses observed in the field, the preferred subsurface conductivity model estimated through inversion is often ambiguous. A central challenge is that a robust stochastic model exploration in 3D, while conceptually the best way to expose such ambiguity, is too computationally demanding to be used as a standard practice. Consequently, most studies report a single deterministic model, which obscures the range of alternative geological structures that are equally consistent with the data.

In this work we propose a practical approach to stochastic model exploration in 3D MT inversion. Drawing inspiration from annealing methods, we adopt a Very Fast Simulated Annealing (VFSA) framework, with sparse parameterization that makes the optimisation feasible for large-scale problems. Our inversion algorithm is built around the widely used ModEM forward solver, ensuring compatibility with existing workflows. Instead of producing one definitive model, the workflow can generate a set of plausible models that explain the data equally well. From this ensemble one can compute statistical summaries: a mean model that captures the most consistent structures and quantitative measures of variability that highlight where geometry, depth, or connectivity remain uncertain. This representation enables geologists to make interpretations while being explicitly aware of the uncertainty inherent in the inversion.  We demonstrate that the approach works at regional scale using a large-area subset of USArray MT data from Cascadia. This dataset has been extensively studied and previously modelled with deterministic 3D inversion, which allows us to benchmark our results.

How to cite: Mishra, P. K., Kamm, J., Patzer, C., Autio, U., and Sen, M. K.: Building uncertainty-aware subsurface models with 3D magnetotelluric inversion, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4367, https://doi.org/10.5194/egusphere-egu26-4367, 2026.

EGU26-4681 | Posters on site | EMRP2.3

Geoelectrical structure beneath the epicentral area of the 2016 Gyeongju earthquake, southeastern Korea, from magnetotelluric data 

Kiyeon Kim, Seokhoon Oh, Hyoung-Seok Kwon, Seong Kon Lee, and Kyeongho Ryu

Southeastern Korea is transected by the Yangsan Fault System, a major fault network comprising numerous faults developed around the Yangsan Fault. In September 2016, a ML 5.8 earthquake occurred in the Gyeongju area along the Yangsan Fault, with a focal depth of ~12–16 km. This event represents the largest instrumentally recorded earthquake in South Korea, which is located in an intraplate tectonic setting. Given the complex fault geometry and stratigraphy of the Gyeongju area, imaging the deep subsurface structure is essential for understanding the seismotectonic framework.

We conducted three-dimensional (3D) inversion of magnetotelluric (MT) data from 120 sites in the epicentral area and interpreted the resulting geoelectrical structure. The resistivity model delineates high-resistivity zones corresponding to granitoids and volcaniclastic rocks, whereas low-resistivity zones are consistent with sedimentary rocks and Quaternary alluvial deposits. This correspondence indicates that the geoelectrical structure reflects regional lithologic variations. At depths corresponding to the hypocentral range, a pronounced low-resistivity anomaly is resolved, and the 2016 Gyeongju earthquake is interpreted to have occurred beneath this conductive body. These results indicate that the deep geoelectrical structure beneath the Gyeongju area is characterized by distinct conductive and resistive features. In future studies, a multidisciplinary approach is needed for a reliable, integrated interpretation of the seismotectonic framework.

How to cite: Kim, K., Oh, S., Kwon, H.-S., Lee, S. K., and Ryu, K.: Geoelectrical structure beneath the epicentral area of the 2016 Gyeongju earthquake, southeastern Korea, from magnetotelluric data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4681, https://doi.org/10.5194/egusphere-egu26-4681, 2026.

EGU26-5214 | ECS | Orals | EMRP2.3

Weak-Signal Reconstruction under Strong Noise in Borehole Transient Electromagnetics 

Yi Ye, Chao Zhang, and Nian Yu

The borehole transient electromagnetic (BTEM) method is a key technology for metallic mineral, groundwater, and related resource exploration, with measured responses exhibiting exponential decay over multiple orders of magnitude in dynamic range. However, late-time signals attenuate to extremely low amplitudes and become submerged in noise, creating a bottleneck for exploration depth. To address the limitations of conventional processing approaches under low signal-to-noise ratio conditions, we propose a reconstruction framework that exploits the non-stationary nature and time–frequency evolution of BTEM decay curves. The framework incorporates two complementary mechanisms. A time–frequency ultra-pyramid fusion module captures the evolving decay behavior in the time–frequency domain and enables robust separation of signal and noise. In parallel, a noise-aware gating mechanism learns point-wise reliability weights from feature statistics to regulate activations, suppressing noise-dominated late-time components while retaining informative signal content. Validation on synthetic and field datasets demonstrates that the proposed approach extends the effective observation window and reliably recovers weak signals from the noise floor, thereby enhancing the achievable exploration depth for BTEM.

How to cite: Ye, Y., Zhang, C., and Yu, N.: Weak-Signal Reconstruction under Strong Noise in Borehole Transient Electromagnetics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5214, https://doi.org/10.5194/egusphere-egu26-5214, 2026.

EGU26-5546 | ECS | Posters on site | EMRP2.3

3D numerical model for investigating the effect of relative magnetic permeability in magnetotellurics 

Renáta Szebenyi, Attila Galsa, and János Kiss

This work concerns the construction and testing of a 3D numerical model suitable for the simulation of magnetotelluric measurements using COMSOL Multiphysics. The aim of the study is to inspect the effect of varying relative magnetic permeability of rocks (different from the general approximation of 1) and integrate it to geology based numerical models.

Experiences from field magnetotelluric (MT) measurements indicate that in the vicinity of igneous rocks field MT data shows increased resistivities at lower frequencies. This effect may be connected to the rocks’ magnetic susceptibility/permeability which differ from these parameters of vacuum and are generally neglected (e.g. Li & Cao 2005, Kiss et al. 2023). The presence of media with relative magnetic permeability higher than 1 may affect the depth estimation during data processing and interpretation (Kiss et al. 2023). In this study, we investigate these effects in detail applying a model to a real geological research area in Hungary to find possible explanations of the behaviour of measured MT data.

First, 1-, 2-, and 3-layer synthetic models were created to test several model parameters and verify numerical results with the analytical solutions of the respective models. Parameter tests included the size of the model, the frequency range, the resistivity and thickness of the “air” domain, the resistivity contrast of the layers, and the mesh resolution. As a result, numerically accurate models were gained: the difference between the numerical results and the analytical ones were less than 0.05% for the apparent resistivity and less than 0.3% for the phase.

Second, the effect of the relative magnetic permeability was studied. Values were chosen to range from 1 to 10. Larger values allowed us to examine the effect of the physical phenomenon, while smaller values provided information on the potential extent of the effect in reality. In the model 11 simulated measurement points were distributed along a line, 1 km apart from each other. Several models were created where the boundary of the regions with different permeability values was perpendicular to the “measurement line” or was located at an angle to the line.

Third, a model was built based on the real geology of a study area near Székesfehérvár, Hungary, where the Pre-Cenozoic basement consists of granitoid plutons and siliciclastic and carbonate formations covered by Miocene sedimentary rocks. Preliminary results of real magnetotelluric field measurements and the modelled ones were compared. It was established that the numerical model results harmonize with field observations, but further refinements are needed.

 

References:

X.M. Li & J.X. Cao (2005): A study on the influence of magnetic susceptibility on MT response. Chinese Journal of Geophysics, 48(4):1017-1021

Kiss, L. Szarka & E. Prácser (2023): Magnetic distortions in magnetotellurics: Predictable distortions in classical processing MT procedures in presence of a magnetic medium based on 2D direct modelling results (in Hungarian). Hungarian Geophysics, 64(1):43-57

How to cite: Szebenyi, R., Galsa, A., and Kiss, J.: 3D numerical model for investigating the effect of relative magnetic permeability in magnetotellurics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5546, https://doi.org/10.5194/egusphere-egu26-5546, 2026.

Submarine hydrothermal vents associated with active volcanoes provide valuable insight into the shallow fluid migration pathways and volatile transport from magmatic systems. The distribution and activity of these vents are controlled by the subseafloor structure such as faulting and zones of hydrothermal alteration. These structural features govern fluid pathways and influence long-term volcanic behavior making the location, geometry, and variability of these structural and alteration features important information for volcanic hazard assessment. Additionally, hydrothermal vents provide sources of heat and chemically distinct substrates that support benthic ecosystems. Identifying and characterizing these features aids better understanding and management of these ecosystems.

Controlled-source electromagnetic (CSEM) methods are well suited for investigating these systems due to their sensitivity to changes in electrical resistivity associated with pore fluid composition and hydrothermal alteration. Here, we present results from a surface-towed CSEM survey conducted offshore Whakaari/White Island in the Taupō Volcanic Zone, New Zealand. The survey targeted regions containing previously mapped vent sites and was designed to image hydrothermal pathways within the upper few hundreds of meters of the seafloor. Additionally, survey lines extended from the island to the area surrounding Te Paepae o Aotea/Volkner Rocks, a site of inferred structural and magmatic connectivity, to capture active hydrothermal vent sites or shallow subseafloor alteration associated with prior venting activity.

Preliminary inversions reveal electrical resistivity signatures that we interpret as zones of volcanically altered material, fluid and/or gas flow along fault structures, and individual vent features. These results provide a detailed view of near-seafloor electrical structure associated with active and relict hydrothermal processes offshore Whakaari. Our inversions complement deeper constraints on magmatic systems from ocean-bottom EM surveys and regional airborne EM data by resolving shallow conductive and resistive features linked to fluid flow and alteration. These data improve characterization of shallow subsurface structure and hydrothermal pathways in an active volcanic setting and demonstrate the sensitivity of surface-towed CSEM to vent-related processes in the shallow seafloor.

How to cite: King, R., Miller, C., and Constable, S.: Imaging Submarine Faulting, Hydrothermal Alteration, and Vent Structures Offshore Whakaari/White Island Using Surface-Towed Controlled Source Electromagnetics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5746, https://doi.org/10.5194/egusphere-egu26-5746, 2026.

EGU26-6356 | Posters on site | EMRP2.3

Three-dimensional resistivity model of the southeastern part of Gangwon Province, Korea, using integrated AMT and electrical resistivity surveys 

Seong Kon Lee, Hyoung-Seok Kwon, Kiyeon Kim, Seokhoon Oh, Manho Han, and Soocheol Jeong

We present a three-dimensional (3D) geological model of the south-eastern Gangwon Province, Korea, using integrated geophysical datasets. The study area has historically hosted numerous coal and metal mines, many of which are now abandoned. Recently, renewed interest in critical minerals has driven active mineral exploration. In addition, the area has been selected as a potential site for underground research laboratory for high-level radioactive waste disposal and cosmic particle research. 

In this study, audio-magnetotelluric (AMT) data acquired at grid-distributed measurement stations were analyzed. A total of 49 AMT survey stations were deployed in a generally non-uniform grid configuration. Measurement stations were densely distributed at approximately 100 m intervals around the candidate site for underground research facility, while station spacing increased to approximately 250–350 m toward the outer areas. For remote reference measurements, a remote reference station was operated at a distance of approximately 12–14 km from the survey area.

Three north–south profiles, three east–west profiles, and additional virtual two-dimensional profiles oriented in the northeast–southwest and northwest–southeast directions were defined. Two-dimensional inversion was performed along these profiles to obtain a preliminary geological model for subsequent 3D inversion. These models, together with two-dimensional inversion results derived from electrical resistivity survey lines, were used as initial models to facilitate faster convergence in 3D inversion. Furthermore, near-surface electrical resistivity obtained from inversion of electrical resistivity data was incorporated into the initial model to minimize static effects caused by by near-surface resistivity inhomogeneities.

The geological model derived from the 3D inversion was validated through comparison with airborne magnetic survey data and available borehole information from the study area. Continuity of geological features, including coal seams and lithological boundaries between limestone and granite, was confirmed on individual two-dimensional sections, leading to the construction of a new 3D geological model. The developed 3D resistivity model provides a reliable geophysical framework for mineral exploration and for site characterization of underground research facilities in this region.

How to cite: Lee, S. K., Kwon, H.-S., Kim, K., Oh, S., Han, M., and Jeong, S.: Three-dimensional resistivity model of the southeastern part of Gangwon Province, Korea, using integrated AMT and electrical resistivity surveys, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6356, https://doi.org/10.5194/egusphere-egu26-6356, 2026.

EGU26-6947 | ECS | Posters on site | EMRP2.3

3D Magnetotelluric Inversion Using Levy Gradient Descent Scheme 

Ziyu Tang, Bo Yang, and Yi Zhang

Geophysical inversion algorithms can be categorized into gradient-based quasi-linear inversion and stochastic-search-based fully nonlinear inversion. Quasi-linear methods, such as gradient descent and conjugate gradient, rely on the gradient information of the objective function with respect to the model parameters for updates. These methods are prone to getting trapped in local minima and lack quantitative methods for evaluating inversion results. Fully nonlinear inversion methods, such as genetic algorithms and Monte Carlo methods, search the solution space through various stochastic processes, offering the advantage of avoiding local minima. However, they incur excessively high computational costs in 3D scenarios, making them difficult to apply to field data at present. We propose the Levy Gradient Descent (L-GD) method based on the Levy flight process and explore its performance in 3D magnetotelluric (MT) inversion.

The Levy flight process, derived from the Levy distribution introduced by the French mathematician Paul Lévy, is a random walk process that combines high-frequency small steps with low-frequency large steps. The heavy-tailed characteristic of Levy flights demonstrates unique advantages in escaping local minima and extensively exploring the solution space, making it highly suitable for solving large-scale complex optimization problems. This makes the L-GD algorithm a highly promising semi-stochastic search-driven algorithm. We have implemented the 3D MT L-GD inversion algorithm based on the open-source ModEM framework. Building upon this existing codebase, we integrated an inversion module based on the L-GD algorithm. Furthermore, we accelerated the forward modeling process using the cuBiCG solver developed by Dong et al. (2024) on GPU, transforming it into a practical 3D MT inversion method. Additionally, traditional methods typically rely solely on the RMS data misfit to evaluate the final inversion result. To provide model evaluation criteria beyond data misfit, we calculate statistical information for models along the search path, obtaining the mean and standard deviation of all models during the inversion iterations. This statistical information is essentially a weighted combination of gradients, reflecting the characteristics of the marginal distribution for each parameter in the high-dimensional solution space, thereby providing crucial indirect information for the reliability analysis of the optimal model.

We conducted a series of synthetic and field data tests on the L-GD algorithm. The results indicate that this algorithm can achieve better data misfit compared to the NLCG algorithm, and the model statistical information provides intuitive reference for evaluating the optimal model. Furthermore, our experiments demonstrate that for semi-stochastic inversion algorithms like L-GD, the traditional cooling method—which gradually reduces the regularization factor of the model constraint term during iterations—is not conducive to obtaining better inversion results. Instead, fixing the regularization factor at a small, low value proves to be a superior strategy.

This research was supported by grants from National Major Science and Technology Projects of China: Deep Earth Probe and Mineral Resources Exploration (2024ZD1000200) and National Natural Science Foundation of China General Program (42474103).

How to cite: Tang, Z., Yang, B., and Zhang, Y.: 3D Magnetotelluric Inversion Using Levy Gradient Descent Scheme, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6947, https://doi.org/10.5194/egusphere-egu26-6947, 2026.

The horizontal magnetic inter-station transfer function (hereinafter referred to as M) establishes the relationship between horizontal magnetic fields at the local site and the reference site (Hl = MHr). 3D numerical simulation (Wen et al., in revision) indicates that M can effectively mitigate the "speckle-shaped artifacts" in shallow structures often observed in the inversion of long-period sparse arrays, and improve the recovery effect of the lateral boundaries of high-conductivity anomalies. Incorporating M data from a synchronized sub-array into the inversion, alongside the traditional impedance tensor (Z) and tipper (T), holds significant potential for enhancing the resolution of shallow electrical structures.

To verify the above conclusions and evaluate the practical application of M in complex geological environments, we conducted imaging of field data containing M data in the Bayan Obo area, Inner Mongolia, China. This region is located in the transition zone between the Yinshan Orogenic Belt and the North China Craton, characterized by significant lateral heterogeneity, making it an ideal site for testing resolution characteristics. We deployed an MT array with varying station spacings. While constructing a high-resolution reference model using the inversion of the dense station dataset, we also conducted inversion experiments on the sparse station data from multiple subsets of this dataset. By comparing the results of Z+T inversion with Z+M joint inversion, we verified and quantified the resolution capability of M for shallow electrical structures. Furthermore, by selecting sites with different electrical structures within the survey area as reference stations, we tested the impact of the subsurface electrical structure beneath the reference station on the resolution capability of M.

This research was supported by grants from National Major Science and Technology Projects of China: Deep Earth Probe and Mineral Resources Exploration (2024ZD1000200) and National Natural Science Foundation of China General Program (42474103).

How to cite: Chen, D., Yang, B., Wen, G., and Wu, X.: Three-dimensional magnetotelluric imaging including inter-station transfer function in Bayan Obo region, Inner Mongolia, China, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7264, https://doi.org/10.5194/egusphere-egu26-7264, 2026.

The Xiaojiang fault is a large active fault and a strong earthquake zone with strong tectonic motion. Located near the middle zone of the Emeishan Large Igneous Province and as the southeastern boundary of the Tibetan Plateau, it plays an indispensable role in the lateral escape mechanism of plateau material and regional tectonic evolution. Previous studies have shown that the Xiaojiang fault has low velocity, high Poisson's ratio, low electrical resistivity, high heat flow, and strong attenuation, while the Emeishan Large Igneous Province inner zone has high velocity, high electrical resistivity, and low heat flow. The location and morphology of channel flow are still inconclusive. The magnetic susceptibility structure obtained from regional magnetic anomalies can directly reveal the deep magnetic structure, while the thermal structure is direct evidence to support the material transport. This report aims to study the thermal structure of the Xiaojiang fault and its surrounding areas. Combined with the previous research to identify heat flow channels, determine the possible places of crust-mantle material exchange, clarify the material transport mechanism, and explore the regional seismic hazard. This report aims to provide a diversified supplement to the deep material structure and material transport mechanism in this region, and to understand the deeper geoscientific significance of the Xiaojiang fault and its surrounding area.

How to cite: Dong, C.: The Deep Material Structure of the Xiaojiang Fault and Its Surrounding Areas: Based on Magnetic Anomaly Model and Magnetotelluric Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8629, https://doi.org/10.5194/egusphere-egu26-8629, 2026.

EGU26-8800 | Posters on site | EMRP2.3

Three-dimensional magnetotelluric Bayesian inversion based on Stein variational gradient descent 

Zehan Liao, Hao Yang, Xin Zhang, Ji Gao, and Haijiang Zhang

To address the challenge of assessing the reliability of three-dimensional (3D) magnetotelluric (MT) inversion results, we have developed a variational inference (VI) inversion framework (VI-MT) based on the Stein Variational Gradient Descent (SVGD) method. Through parallel particle optimization, we efficiently approximate the model posterior distribution, overcoming the computational limitation of traditional Markov Chain Monte Carlo (MCMC) methods. Synthetic test shows the VI-MT inversion results align with deterministic solutions while better recovering resistivity amplitudes. In comparison, the VI-MT inversion can effectively identify large model uncertainties in the boundary region by the associated multimodal posterior characteristics. Furthermore, the VI-MT inversion is applied to the field MT data collected at the Weishan volcano in northeast China, with the posterior mean model consistent with the deterministic inversion model. Depth-dependent model uncertainties indicate strong data constraints in the upper crust. A clear low resistivity body of ~5 Ω·m with small uncertainties is imaged at depths of ~2-6 km beneath the volcanic crater, suggesting the existence of a shallow magma chamber. Our study shows that the VI-MT inversion based on the SVGD method can efficiently solve the 3D MT Bayesian inversion, providing reliable model uncertainties.

How to cite: Liao, Z., Yang, H., Zhang, X., Gao, J., and Zhang, H.: Three-dimensional magnetotelluric Bayesian inversion based on Stein variational gradient descent, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8800, https://doi.org/10.5194/egusphere-egu26-8800, 2026.

EGU26-10787 | ECS | Posters on site | EMRP2.3

Analysis of Magnetotelluric and Gravity Anomaly Datasets in the Bakony-Balaton Highland Volcanic Field 

Tibor Rubóczki, Jan Vozár, Jaroslava Pánisová, Thomas Lange, Barbély Enikő, and Márta Berkesi

The Bakony-Balaton Highland Volcanic Field (BBHVF) is one of the most geodynamically complex regions within the Pannonian Basin. Based on legacy telluric and magnetotelluric surveys, it has been hypothesized that regions of high electrical conductivity dominate at crustal depths beneath this Neogene volcanic field. Several theories have been proposed to explain their existence, ranging from the localized presence of highly conductive graphite to the role of deep fluid upwelling. The objective of this study is to analyze newly available long-period magnetotelluric datasets using 2D and 3D inversion techniques and to model the Bouguer gravity anomalies of the area by 3D forward density modeling method. Furthermore, we analyze the information directly derivable from MT response functions to draw fundamental geological and petrophysical conclusions. This investigation aims to fill a gap by reviewing earlier geophysical interpretations that are still debated. The goal is to see which geological explanation is more likely, the presence of a specific solid component with high conductivity or the flow of deep fluids linked to the Neogene volcanic field.

How to cite: Rubóczki, T., Vozár, J., Pánisová, J., Lange, T., Enikő, B., and Berkesi, M.: Analysis of Magnetotelluric and Gravity Anomaly Datasets in the Bakony-Balaton Highland Volcanic Field, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10787, https://doi.org/10.5194/egusphere-egu26-10787, 2026.

EGU26-11412 | ECS | Orals | EMRP2.3

Magnetotelluric imaging of a low-enthalpy geothermal system in the Lough Neagh Basin, Northern Ireland 

Dieno Diba, Duygu Kiyan, Colin Hogg, Giuseppe Maggio, Christopher Bean, Derek Reay, Michael MacKenzie, Michelle O'Grady, and Marie Cowan

Sedimentary basins in Northern Ireland are increasingly recognised as promising targets for low- to medium-temperature geothermal energy, yet their subsurface architecture and reservoir properties remain poorly constrained. The Lough Neagh Basin exhibits elevated geothermal gradients relative to other regions of Ireland and represents a low-enthalpy, sedimentary-basin geothermal system. The basin is known to contain sedimentary rocks ranging from at least Permian to Upper Cretaceous in age, overlain by thick Paleogene basalts. Within this system, the electrically conductive Triassic Sherwood Sandstone Group is considered the principal geothermal reservoir, although deeper Permian sandstone units may also have reservoir potential.

In this study, we assess the geothermal potential of the Lough Neagh Basin using a broadband magnetotelluric (MT) dataset comprising more than 250 MT stations, including 118 newly acquired stations as part of the GEMINI (Geothermal Energy Momentum on the Island of Ireland) project. MT data were processed to derive impedance tensors and vertical magnetic transfer functions, followed by phase tensor and induction arrow analyses to characterise dimensionality and lateral resistivity variations. Three-dimensional (3-D) MT inversion was then applied to recover the subsurface resistivity structure.

The resulting 3-D resistivity structure reveals laterally extensive low-resistivity zones with a spatially variable upper boundary, typically initiating at depths of ~0.7–1.0 km and extending to ~2–2.5 km beneath a high-resistivity basalt sequence. These zones are interpreted as the Triassic Mercia Mudstone Group–Sherwood Sandstone Group succession with variable thickness, consistent with borehole constraints and regional geological understanding. While MT primarily constrains the geometry of this conductive package, integration with petrophysical measurements from selected rock samples and other geophysical datasets (i.e., gravity and passive seismics) aids discrimination between mudstone- and sandstone-dominated intervals, enabling first-order estimates of reservoir geometry and associated heat capacity within the Lough Neagh Basin geothermal system.

How to cite: Diba, D., Kiyan, D., Hogg, C., Maggio, G., Bean, C., Reay, D., MacKenzie, M., O'Grady, M., and Cowan, M.: Magnetotelluric imaging of a low-enthalpy geothermal system in the Lough Neagh Basin, Northern Ireland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11412, https://doi.org/10.5194/egusphere-egu26-11412, 2026.

EGU26-11849 | ECS | Orals | EMRP2.3

Two-dimensional Magnetotelluric Inversion using Optimal Transport and Automatic Differentiation  

xinran liu, Xuanzhang Chen, Ziyu Tang, and Yang Bo

Magnetotelluric (MT) data inverse problem is inherently characterized by strong non-linearity. Consequently its solution using the conventional gradient-based algorithm is highly dependent on the initial model. Usually, conventional inversion schemes (e.g. Non-linear Conjugate Gradient, NLCG) employ L₂ norm to form the objective function, measuring the data misfit. However, this metric often fails to capture the phase shifts and global structural features of complex response curves, causing the inversion iteration to become easily trapped in local minima. To address this challenge, we propose a novel 2D MT inversion framework based on Optimal Transport (OT) theory, introducing the Wasserstein distance (W₂) as a robust misfit measure.

We represent the MT dataset as a six-dimensional point cloud within a joint space-feature domain. In this framework, frequencies and station coordinates constitute the spatial dimensions, while the multi-modal responses—including apparent resistivity and phase for both TE and TM modes—form the feature dimensions. By incorporating coordinates and frequencies into the distance computation, the W₂ metric effectively constrains the overall morphological evolution of the response curves across both spatial and spectral domains, providing stronger geometric and topological constraints than the L₂ norm. We implemented the algorithm using the GeomLoss library and PyTorch, leveraging entropy-regularized Sinkhorn distances and Automatic Differentiation (AD) for efficient and precise gradient computation.

Numerical experiments on 2D synthetic models demonstrate that the OT-based inversion exhibits superior convergence stability compared to traditional methods, particularly under demanding conditions where the initial model significantly deviates from the ground truth. Furthermore, the proposed method maintains high resolution for deep conductive anomalies, even under significant noise levels. These results indicate that treating MT data as high-dimensional point clouds within an Optimal Transport framework provides a robust, geometry-sensitive, and innovative technical path for geophysical imaging.

This research was supported by grants from National Major Science and Technology Projects of China: Local Funds for the "Double First-Class" Initiative (924041), Deep Earth Probe and Mineral Resources Exploration (2024ZD1000200) and National Natural Science Foundation of China General Program (42474103).

 

How to cite: liu, X., Chen, X., Tang, Z., and Bo, Y.: Two-dimensional Magnetotelluric Inversion using Optimal Transport and Automatic Differentiation , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11849, https://doi.org/10.5194/egusphere-egu26-11849, 2026.

EGU26-11889 | Orals | EMRP2.3

Present-Day Architecture of the Magma Plumbing System beneath Hekla Volcano from Magnetotelluric Imaging 

Duygu Kiyan, Magnus T. Gudmundsson, Knutur Arnason, Olgeir Sigmarsson, Gylfi P. Hersir, Graham Hill, Alexander Grayver, Christopher J. Bean, Cesar Castro, Svetlana Kovacikova, Colin Hogg, Giuseppe Maggio, and Dmitry Molodtsov

Hekla volcano, one of Iceland’s most active stratovolcanoes, is characterised by very short eruption precursory times and a complex tectonic setting at the intersection of the South Iceland Seismic Zone (SISZ) and the Eastern Volcanic Zone. Despite its frequent activity, the geometry and connectivity of the magmatic system beneath Hekla remain poorly constrained. In this study, we use three-dimensional magnetotelluric (MT) imaging to investigate the electrical resistivity structure beneath Hekla and its implications for magma storage and transport.

This study forms part of a newly funded project under the Research Ireland Frontiers for the Future Programme, with objectives to (i) characterise the present-day structure, depth extent, and geometry of the magmatic system beneath Hekla, (ii) identify low-resistivity zones that may serve as proxies for partial melt and magma migration pathways, and (iii) assess potential magmatic interconnection between Hekla and the adjacent Torfajökull volcanic system, including the possibility of a shared deep magma source. Preliminary 3D inversion results based on MT data from 20 broad-band stations reveal two principal conductive features. Shallow (<2 km) N–S-trending conductive anomalies are observed beneath and southeast of the central edifice. These features are interpreted as groundwater-saturated fracture networks associated with regional faulting within the SISZ. At greater depths (approximately 6–24 km), a pronounced NW–SE-oriented conductive body is imaged beneath Hekla, oriented obliquely relative to the ENE-trending surface fissure swarm. This deeper anomaly is interpreted as a magma storage zone and may play a key role in controlling Hekla’s eruptive behaviour and rapid unrest development. In 2025, the MT network was expanded with data from over 30 additional stations, significantly improving spatial coverage and resolution. This contribution presents the newly acquired data and integrated 3D inversion results combining the new and existing datasets, providing enhanced constraints on the crustal-scale magmatic architecture beneath Hekla and its relationship to regional tectonic structures.

How to cite: Kiyan, D., Gudmundsson, M. T., Arnason, K., Sigmarsson, O., Hersir, G. P., Hill, G., Grayver, A., Bean, C. J., Castro, C., Kovacikova, S., Hogg, C., Maggio, G., and Molodtsov, D.: Present-Day Architecture of the Magma Plumbing System beneath Hekla Volcano from Magnetotelluric Imaging, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11889, https://doi.org/10.5194/egusphere-egu26-11889, 2026.

The Ni–Cu sulphide mineralisation investigated in this study is hosted within a steeply dipping, differentiated ultramafic sill composed primarily of tremolite schist and lenticular bodies of harzburgite. The harzburgite contains net-textured sulphides and occasional massive sulphide veins, with mineralisation dominated by pyrrhotite, chalcopyrite, and pentlandite. Physical property measurements indicate that the mineralised sill is both more conductive and magnetically susceptible than the surrounding country rocks, making it a viable target for geophysical inversion.


This study integrates airborne magnetic data, ground and downhole electromagnetic (EM) surveys, and audio-frequency magnetotelluric (AMT) data to map discontinuous sulphide-rich harzburgite bodies. Magnetic and EM modelling techniques were used to delineate high-conductance zones, which were integrated with geological models to highlight potential extensions of mineralised pods. AMT inversion further confirmed the geometry of the mineralised intrusion. The results demonstrate the value of combining multiple geophysical methods to guide drilling and improve targeting of discontinuous sulphide-rich bodies within ultramafic systems.

How to cite: Mapuranga, V. and Ushendibaba, M.: Mapping discontinuous sulphide-rich harzburgite bodies using geophysical inversion techniques: A case study from a Ni–Cu deposit, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12604, https://doi.org/10.5194/egusphere-egu26-12604, 2026.

EGU26-15114 | ECS | Orals | EMRP2.3

Implicit neural representation for Magnetotelluric inversion  

Yanyi Wang, Xavier Garcia, Eric Attias, Zhenwei Guo, and Boyao Zhang

Magnetotelluric (MT) data inversion aims to recover subsurface resistivity model by minimizing an objective function, typically comprising a data misfit term and a regularization term (e.g., Tikhonov-style regularization). While gradients-based optimization is widely used, it is prone to local minima and highly sensitive to the initial model. In contrast, nonlinear stochastic algorithms explore a broader solution space but are computationally prohibitive for large-scale MT problems.

Deep learning (DL) has emerged as a powerful alternative. Unlike purely data-driven methods, physics-driven DL frameworks embed physical laws, such as wave propagation equation and Maxwell’s equation, as constraints, enhancing interpretability and reducing the need for massive datasets. Implicit neural representation (INR) is a novel physics-driven technique that represents physical properties as continuous functions of spatial coordinates. A key advantage of INR is its inherent ‘frequency principle’ (or spectral bias), where the network learns large-scale (low-frequency) structures before fine-tunning high-resolution (high-frequency) details. In MT inversion, this bias acts as an implicit regularization, improving stability without requiring manually tuned penalty terms.

In this paper, we propose an INR-based 2D MT inversion algorithm. Synthetic tests on block and layered models demonstrate that the proposed method recovers anomalous boundaries with higher resolution than traditional Occam-based inversions. Finally, application to the COPROD2 field dataset confirms the practical robustness of the approach and its potential for extension to three-dimensional, mesh-free inversions.

How to cite: Wang, Y., Garcia, X., Attias, E., Guo, Z., and Zhang, B.: Implicit neural representation for Magnetotelluric inversion , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15114, https://doi.org/10.5194/egusphere-egu26-15114, 2026.

EGU26-15506 | ECS | Posters on site | EMRP2.3

The Uplift Mechanism of the Eastern Himalayan Syntaxis 

Gang Wang, Hui Fang, and Fagen Pei

The Eastern Himalayan Syntaxis (EHS) has undergone intense crustal shortening, giving rise to spectacular topography in the Tibetan Plateau. Several tectonic models have been proposed to explain its deformation, including crustal-scale folding, indenter corner dynamics, and tectonic aneurysm mechanisms. Understanding the crustal architecture and present-day state of the EHS is essential for deciphering its tectonic evolution. We deployed a 100-km-long magnetotelluric profile across the Eastern Himalayan Syntaxis and performed three-dimensional inversion of the acquired data, yielding a high-resolution 3D electrical model that finely constrains the crustal structure and material state. Based on this model, we analyzed the crustal material conditions, estimated partial melt fractions, and assessed crustal rheology. Integrating our results with complementary geophysical and petrological evidence, we found that crustal materials on the northwestern side of the EHS show extensive partial melting, indicative of channel flow or upward migration of hot material. In contrast, the southeastern side exhibits pronounced strike-slip characteristics. Thus, the rapid uplift of the EHS appears to result primarily from a combination of crustal partial melting within the syntaxis and intense erosion by the Yarlung Tsangpo Gorge.

How to cite: Wang, G., Fang, H., and Pei, F.: The Uplift Mechanism of the Eastern Himalayan Syntaxis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15506, https://doi.org/10.5194/egusphere-egu26-15506, 2026.

EGU26-17202 | Posters on site | EMRP2.3

3D Audio-Magnetotelluric Imaging of the Aeolian Islands for Geothermal Resource Assessment 

Antonio Troiano, Maria Giulia Di Giuseppe, Roberto Isaia, Pietro Boni, Claudio De Paola, Alessandro Fedele, Gino Gonzalez, Fabio Pagiara, and Monica Sposato

The Aeolian Archipelago (southern Italy) hosts several active volcanic islands characterised by widespread hydrothermal manifestations and represents a strategic natural laboratory for assessing geothermal resources in insular volcanic settings. In such environments, Audio-Magnetotelluric (AMT) surveys are particularly effective for imaging shallow geothermal systems, as electrical resistivity is highly sensitive to fluid content, temperature, and hydrothermal alteration. Moreover, AMT data provide key constraints on major structural discontinuities that control fluid circulation at depth.

This study presents the results of a large-scale geophysical investigation conducted across the islands of Lipari, Salina, Vulcano, and Panarea, with the aim of providing a geophysically constrained assessment of geothermal resources at the scale of the entire archipelago. The focus is on the application of three-dimensional AMT resistivity imaging, which allows detailed characterization of subsurface electrical properties and offers insights into hydrothermal alteration patterns, fluid pathways, and the structural framework relevant for geothermal exploration.

The resulting 3D resistivity models reveal marked lateral and vertical variability in subsurface electrical structure among the investigated islands. These differences reflect contrasting degrees of geothermal system development, variations in fluid circulation regimes, and the role of island-specific structural controls. Rather than indicating a uniform geothermal architecture across the Aeolian Archipelago, the models highlight distinct resistivity patterns and geothermal signatures for each island, emphasizing the heterogeneity of volcanic and hydrothermal processes at the regional scale.

Overall, this study demonstrates the effectiveness of AMT resistivity imaging in discriminating between different geothermal settings and in identifying structural controls on fluid circulation in complex volcanic island environments. The results provide a robust geophysical contribution to the construction of an archipelago-scale inventory of geothermal resources and establish a solid basis for future integration with geological, geochemical, and complementary geophysical datasets. This integrated approach is essential for informed evaluation and modelling of sustainable geothermal exploitation scenarios in the Aeolian Islands

How to cite: Troiano, A., Di Giuseppe, M. G., Isaia, R., Boni, P., De Paola, C., Fedele, A., Gonzalez, G., Pagiara, F., and Sposato, M.: 3D Audio-Magnetotelluric Imaging of the Aeolian Islands for Geothermal Resource Assessment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17202, https://doi.org/10.5194/egusphere-egu26-17202, 2026.

EGU26-21012 | Posters on site | EMRP2.3

Extending MARE2DEM to Semi-Airborne and Full Airborne EM Inversion: Synthetic Validation  

Shunguo Wang, Marin Yanev, and Vikas Chand Baranwal

MARE2DEM (Modeling with Adaptively Refined Elements for 2-D EM) is a freely available 2-D inversion code originally developed by Dr. Kerry Key for marine electromagnetic (EM) surveys. Since the code is open-source, other researchers have extended it to new domains. This demonstrates the flexibility of MARE2DEM for different survey environments beyond its initial marine focus.

In this study, we adapted MARE2DEM to invert semi-airborne and full airborne EM data. The semi-airborne configuration consists of a grounded electric or magnetic dipole transmitter on land with magnetic field receivers flown in air (operating in the ~1–12 kHz band). The inversion results for the semi-airborne case successfully imaged all the detailed structures in the synthetic resistivity models when the recording locations are within 15 m height, confirming that MARE2DEM performs robustly for this new application. Such semi-airborne surveys are well-suited for our targets, such as quick clay deposits and mineral deposits.

By contrast, the full airborne EM case proved challenging. We applied MARE2DEM to a helicopter-borne frequency-domain system (NGU’s “Hummingbird” system) operating at five frequencies (approximately 880 Hz, 6.6 kHz, 34 kHz in horizontal coplanar, and 980 Hz, 7 kHz in vertical coaxial mode) with 5-6 m transmitter–receiver separations. In this scenario, where both transmitter and receivers are airborne and moving, we encountered inaccuracies in the forward modelling. High-frequency airborne EM data are particularly numerically demanding to model it accurately, as the free-space transmitter geometry and high frequency range require very fine discretization. We found that the standard adaptive meshing in MARE2DEM needed further refinement to capture the decaying fields in air. To improve the forward accuracy, we tested a range of strategies, including using more finely discretized meshes and carefully tuning the wavenumber sampling for the 2.5D solver. These measures reduced the modelling errors, but we still did not reach the same level of accuracy for full airborne modelling as in the marine or semi-airborne cases. The results indicate that additional developments are required for full airborne EM data modelling and inversion. In summary, our extension of MARE2DEM works well for semi-airborne EM surveys, achieving resolution comparable to the original marine applications, whereas the full airborne case remains problematic in forward modelling. Further improvements are being explored to enable reliable forward modelling and inversion of full airborne EM datasets.

How to cite: Wang, S., Yanev, M., and Baranwal, V. C.: Extending MARE2DEM to Semi-Airborne and Full Airborne EM Inversion: Synthetic Validation , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21012, https://doi.org/10.5194/egusphere-egu26-21012, 2026.

EGU26-856 | ECS | Orals | EMRP2.6

In-Orbit Calibration of Vectorized Rubidium Magnetometer onboard COSMO 

Tzu-Hsun Kao, Carolina Chism, Oliver Kaplan, Michaela Ellmeier, Svenja Knappe, Jeramy Hughes, and Robert Marshall

The University of Colorado Boulder is scheduled to launch the Compact Spaceborne Magnetic Observatory (COSMO), a 6U CubeSat mission at LEO designed to provide high-resolution measurements of the Earth's magnetic field in support of the next-generation World Magnetic Model (WMM), in March 2026. The payload, known as the Vectorize Rubidium Magnetometer (VRuM), is designed to be less than 1U in size and consists of two optical rubidium scalar magnetometers integrated within a triaxial Braunbek coil system and two star trackers. The Braunbek coils are stimulated with modulation currents at distinct frequencies to generate modulation magnetic fields along each axis, allowing for the vector extraction of the Earth’s magnetic field. In combination with the optical scalars and the Braunbek coil system, the VRuM instrument can be self-calibrated and can also measure the vector magnetic field. After the commissioning phase, in-orbit calibrations and tests will be performed. The in-orbit calibrations include vector calibration, heading error calibration, spacecraft bias characterization, and mounting quaternion determination. The vector calibration aims to determine the non-orthogonality of the coils and the magnitude of modulation fields. The heading error calibration characterizes the heading error of the scalars due to the non-alignment between the measured magnetic field and the cell within the scalars. The spacecraft bias test is designed to determine the static magnetic field created by the small amounts of magnetic material around the payload; this bias field has been estimated on the ground as less than 10 nT. The mounting quaternion is a parameter that transfers the coordinates between the coil system and the star trackers. To obtain the most accurate attitude information, the Uncented Kalman filter is applied. This paper outlines the mission design, magnetometer vectorization technique, calibration methods, and plans for in-orbit calibrations in combination with first observations from space.

How to cite: Kao, T.-H., Chism, C., Kaplan, O., Ellmeier, M., Knappe, S., Hughes, J., and Marshall, R.: In-Orbit Calibration of Vectorized Rubidium Magnetometer onboard COSMO, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-856, https://doi.org/10.5194/egusphere-egu26-856, 2026.

EGU26-1448 | Orals | EMRP2.6

Diagnosing thermospheric density uncertainty from LEO satellites using data assimilation 

Isabel Fernandez-Gomez, Stefan Codrescu, Frank Heymann, Claudia Borries, and Mihail V. Codrescu

The growing constellation of low-Earth-orbit satellites allows us to characterize the thermosphere-ionosphere system (TI). One of the most valuable LEO measurements are accelerometer derived neutral density estimates, which play a central role in satellite drag estimations, TI modeling, and space weather operations. Despite their importance, the measurement uncertainty of satellite-derived neutral density for most LEO missions remains unknown. In this study, we use a data assimilation (DA) based framework to diagnose the observation uncertainty directly from neutral density measurements.

Using the Coupled Thermosphere Ionosphere Plasmasphere electrodynamics model (CTIPe) and TIDA, the TI Ensemble Kalman filter data assimilation scheme, we perform controlled experiments with varied assumed uncertainties. Two complementary diagnostics are applied: the Desroziers method, which estimates the effective observation uncertainty required for a self-consistent DA system, and an ensemble-spread method, which isolates the true measurement error by removing model-projected variability from the innovation variance.

We apply both diagnostics to CHAMP, Swarm A/B/C, and GRACE-A/B across low and high solar-activity periods. Results confirm the expected 10–15% uncertainty for CHAMP during quiet conditions, while GRACE (15–35%) and Swarm (25–50%) exhibit larger values, reflecting differences in altitude, solar activity, instrument characteristics, and thermospheric variability. The two methods provide complementary perspectives and the limit of the estimated uncertainty range: Desroziers quantifies the upper bound, and the ensemble-spread method provides the lower bound uncertainty. The framework provides a pathway to systematically quantify uncertainty in current and upcoming LEO missions, supporting improved density models, drag prediction, and space weather services.

How to cite: Fernandez-Gomez, I., Codrescu, S., Heymann, F., Borries, C., and Codrescu, M. V.: Diagnosing thermospheric density uncertainty from LEO satellites using data assimilation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1448, https://doi.org/10.5194/egusphere-egu26-1448, 2026.

EGU26-2624 | Posters on site | EMRP2.6

Thermospheric Wind Longitudinal Variations in the Southern Mid Latitudes 

Qian Wu, Haonan Wu, and Wenbin Wang

Recent thermospheric wind observation by a balloon borne instrument HIWIND over New Zealand in April 2025 combined with ground based Fabry Perot interferometer observations in Brazil provides a good opportunity to examine the longitudinal variations in the southern mid latitude region.   The results showed noticeable longitudinal variations, which could be generated by nonmigrating tides propagating from the lower atmosphere.      HIWIND also provided the first southern hemisphere daytime thermospheric wind observations.     Combined HIWIND data with COSMIC 2 radio occultation observations of ionosphere profiles in the southern hemisphere we will examine the interaction between the ionosphere and thermosphere.   Using the first principle model TIEGCM we simulated the southern hemisphere thermospheric winds and ionosphere profiles to compare with the HIWIND and COSMIC observations.   HIWIND results help to reveal significant discrepancy between observations and simulations and point toward the direction for future improvement of the simulations.

 

How to cite: Wu, Q., Wu, H., and Wang, W.: Thermospheric Wind Longitudinal Variations in the Southern Mid Latitudes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2624, https://doi.org/10.5194/egusphere-egu26-2624, 2026.

EGU26-2836 | Orals | EMRP2.6

The ESA Scout NanoMagSat Mission, a Nanosatellite Constellation to Further Improve Geomagnetic Field and Ionospheric Environment Monitoring and Modeling, on Course for First Launch in 2027 

Gauthier Hulot, Pierdavide Coïsson, Jean-Michel Léger, Lasse B. N. Clausen, John L. Jørgensen, Jose van den Ijssel, Louis Chauvet, Robin Deborde, Maximilien Salinas, Martin Fillion, Sasha Troncy, Thomas Jager, Christian B. Stoltze, Florian Deconinck, Pepe Nieto, Fabrice Cipriani, Massimiliano Pastena, and Jean-Pascal Lejault

Geomagnetic field and ionospheric environment LEO monitoring is presently achieved by the three polar orbiting, two side-by-side and one with relative local time (LT) drift, satellites of the Swarm Earth Explorer ESA constellation launched in November 2013, forming the backbone of a broader constellation now also including the Chinese CSES-1 and CSES-2 missions launched in February 2018 and June 2025, maintained 180° apart on the same Sun-Synchronous orbit, as well as the Chinese MSS-1 41° inclination mission, launched in May 2023. These are currently the only missions carrying an absolute magnetometry payload critical for global field monitoring.

Here, we will present the latest status of the NanoMagSat constellation mission, third small science mission selected for ESA’s new Earth Observation fast track Scout program that taps into New Space. Scout is a new framework (3 years for implementation, cost ≤ 35 M€) by which ESA aims to demonstrate disruptive sensing techniques or incremental science, while retaining the potential to be subsequently scaled up in larger missions or implemented in future ESA Earth Observation programs.

NanoMagSat will cover all LT at all latitudes, with special emphasis on latitudes between 60°N and 60°S, where all LT will be visited within about a month, much faster than is currently achieved. Each 16 U satellite will carry an advanced miniaturized absolute scalar and self-calibrated vector magnetometer with star trackers collocated on an ultra-stable optical bench at the tip of a 3m deployable boom, a compact High Frequency Magnetometer at mid-boom, a multi-Needle Langmuir Probe and dual frequency GNSS receivers on the satellite body. This payload suite will acquire high-precision/resolution oriented absolute vector magnetic data at 1 Hz, very low noise scalar and vector magnetic field data at 2 kHz, electron density data at 2 kHz, and electron temperature data at 1 Hz. GNSS receivers will also allow recovery of top-side TEC and ionospheric radio-occultation profiles. NanoMagSat will start deploying in 2027, with full constellation to be operated for a minimum of three years between 2028 and 2031.

Science objectives will be introduced and the rationale for the choice of the payload and constellation design explained. The planned data products, with their expected performance, will also be described. Special emphasis will be put on the innovative aspects of the mission with respect to previous missions. Finally, possibilities of further expanding the constellation though international collaboration as encouraged by IAGA resolution 2025 n°1 will be discussed.

How to cite: Hulot, G., Coïsson, P., Léger, J.-M., Clausen, L. B. N., Jørgensen, J. L., van den Ijssel, J., Chauvet, L., Deborde, R., Salinas, M., Fillion, M., Troncy, S., Jager, T., Stoltze, C. B., Deconinck, F., Nieto, P., Cipriani, F., Pastena, M., and Lejault, J.-P.: The ESA Scout NanoMagSat Mission, a Nanosatellite Constellation to Further Improve Geomagnetic Field and Ionospheric Environment Monitoring and Modeling, on Course for First Launch in 2027, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2836, https://doi.org/10.5194/egusphere-egu26-2836, 2026.

EGU26-4332 | ECS | Posters on site | EMRP2.6

Ionosphere small-scale magnetic perturbations associated with GPS scintillations in the auroral and cusp regions 

Yangyang Shen, Robert Strangeway, Hao Cao, James Weygand, Jiashu Wu, Jasper Halekas, Stephen Fuselier, Anthony McCaffrey, Pt Jayachandran, Daniel Billett, Christopher Watson, David Miles, John Bonnell, Roger Roglans, and George Hospodarsky

Magnetosphere and ionosphere coupling is largely driven by electromagnetic waves (e.g., Alfven waves) and particle precipitation in the polar cusp and auroral region. Magnetic perturbations (dB) in the ionosphere span scales from >1,000 km across the auroral zone—associated with Region-1 and Region-2 field-aligned currents (FACs)—down to <1 km, approaching the electron inertial length, corresponding to fine-scale auroral arcs (~100 m). These smaller scale dB are often linked to inertial Alfven waves that carry parallel electric fields, accelerate electrons, and produce dynamic auroral structures. During geomagnetic storms, transient currents associated with these small-scale dB can exceed several hundred μA/m2, leading to significant ionosphere total electron content (TEC) perturbations and plasma irregularities that cause GPS scintillations and disrupt communication. However, it remains a challenge to fully understand how these small-scale FACs and associated particle precipitation drive ionosphere irregularities and GPS scintillations. NASA's TRACERS mission, launched on 23 July 2025, offers new opportunities to address this problem. We present initial observations from TRACERS showing coincident small-scale dB, particle precipitation, and strong GPS scintillation events in the nightside auroral and dayside cusp regions.

How to cite: Shen, Y., Strangeway, R., Cao, H., Weygand, J., Wu, J., Halekas, J., Fuselier, S., McCaffrey, A., Jayachandran, P., Billett, D., Watson, C., Miles, D., Bonnell, J., Roglans, R., and Hospodarsky, G.: Ionosphere small-scale magnetic perturbations associated with GPS scintillations in the auroral and cusp regions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4332, https://doi.org/10.5194/egusphere-egu26-4332, 2026.

EGU26-4384 | Posters on site | EMRP2.6

Adaptive AI Forecasting of Thermospheric Neutral Density Tuned to GRACE Data 

Lotte Ansgaard Thomsen and Ehsan Foorotan

Accurate forecasting of Thermospheric Neutral Density (TND) is essential for Low-Earth Orbit (LEO) mission planning, collision avoidance, and orbit determination. Atmospheric drag strongly influences satellite trajectories below 1000 km altitude, making precise density estimates critical for operational safety. Current empirical and physics-based modelsoften show limited skills to capture short-term variability driven by solar and geomagnetic activity. This limitation reduces their accuracy during dynamic space weather conditions and impacts mission planning.

We propose an adaptive machine learning framework using Extreme Gradient Boosting (XGBoost) to predict the systematic deviations from NRLMSISE-2.1 in log space. The model combines GRACE accelerometer-derived TND observations for the years 2009-2017, CODE's global TEC maps, and space weather indices represented by indices such as F10.7 and Ap. Feature engineering incorporates diurnal and seasonal cycles, altitude dependence, and ionosphere-thermosphere coupling. We apply lagged TEC and geomagnetic indices for short-term memory without needing sequential models. This ensures that this approach stays compatible with tabular workflows and keeps them computationally efficient.

A warm-start learning scheme is introduced tofacilitate short-term adaptation through fine-tuning the model with respect to the most recent observations. Validation on the GRACE and Swarm datasets shows an improvement compared to the original NRLMSISE-2.1 model. The reduction in RMSE is approximately 60-70%, and a MAPE improvement of a similar margin is seen under quiet conditions. Storm-time robustness has also been improved. The model performs well when validated on an off-track manner to validate its spatial generalization properties beyond the nominal orbit covered by the GRACE mission. The RMSE reduction is approximately 40%,

These results highlight the potential of AI-driven approaches for operational thermospheric density forecasting. Improved accuracy supports orbit prediction, drag estimation, and space weather applications. The novel framework combines robustness, adaptability, and computational efficiency. This makes it appropriate for integration into real-time mission planning and collision avoidance systems.

How to cite: Thomsen, L. A. and Foorotan, E.: Adaptive AI Forecasting of Thermospheric Neutral Density Tuned to GRACE Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4384, https://doi.org/10.5194/egusphere-egu26-4384, 2026.

EGU26-6038 | ECS | Orals | EMRP2.6

Initial TRACERS Observations of Auroral Electron Precipitation: Case Studies of Diffuse and Discrete Aurora 

Sarah Henderson, Jasper Halekas, Robert Strangeway, Scott Bounds, Ivar Christopher, Aidan Moore, Suranga Ruhunsuri, and David Miles

The Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites (TRACERS) is a recently launched NASA mission focused on investigating how temporal or spatial variations in magnetic reconnection drive cusp dynamics by employing multipoint, high-cadence measurements from two identical spacecraft. TRACERS successfully launched into a Sun-synchronous 590 km orbit around Earth on July 23, 2025. The two spacecraft comprising TRACERS are equipped with identical instrument payloads capable of measuring ions, electrons, and electromagnetic fields within low-Earth orbit. The primary goal of the TRACERS mission is to disentangle temporal and spatial variation of magnetic reconnection and associated processes by employing multipoint measurements within the cusp from two identical spacecraft (TRACERS-1 and -2), which are separated by 10 to 120 seconds. In addition to its primary science goals of examining cusp dynamics, TRACERS is also capable of measuring auroral precipitation and processes with high spatial and temporal resolution. We present initial auroral electron observations from one of the TRACERS spacecraft on October 7, 2025. We observe both discrete and diffuse electron precipitation in two orbits in the northern hemisphere. TRACERS-2 observes numerous inverted-V structures indicative of discrete aurora within the auroral oval and polar cap, as well as within the northern cusp. Hours later, TRACERS-2 observes broadband, diffuse electron precipitation spanning tens of eV to tens of keV across the northern polar cap, indicative of polar rain. We discuss the upstream solar wind conditions during each observation utilizing Wind data, as well as the characteristic energies, pitch angle distributions, and fluxes of each electron population observed by TRACERS-2 during these two observations.

How to cite: Henderson, S., Halekas, J., Strangeway, R., Bounds, S., Christopher, I., Moore, A., Ruhunsuri, S., and Miles, D.: Initial TRACERS Observations of Auroral Electron Precipitation: Case Studies of Diffuse and Discrete Aurora, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6038, https://doi.org/10.5194/egusphere-egu26-6038, 2026.

EGU26-7057 | Posters on site | EMRP2.6

Equinoctial asymmetry in mid-latitude NmF2 noontime peaks: A formation mechanism  

Loredana Perrone and Andrey Mikhaylov

Mid-latitude semiannual noontime NmF2 peaks were analyzed at four Northern Hemisphere stations (Boulder, Rome, Wakkanai, Juliusruh) and two Southern Hemisphere stations (Hobart, Port Stanley). The aeronomic parameters responsible for the observed NmF2 variations were determined by solving an inverse problem of aeronomy using the original THERION method.

On average, the NmF2 peak in autumn is larger than the vernal peak in both hemispheres under solar minimum conditions. This observed difference in NmF2 between the two peaks is attributed to variations in thermospheric parameters that are not directly related to solar and geomagnetic activity. While the vernal peak can occur over a span of three months in both hemispheres, the autumnal peak is confined to a shorter two-month period.

The primary factor influencing the difference between NmF2 in the two peaks is the abundance of atomic oxygen [O]. A distinct two-hump NmF2 variation, with a trough in December–January in the Northern Hemisphere, reflects a lower concentration of [O] during this period compared to October–November. This variation is driven by changes in [O] rather than by the solar zenith angle effect.

The empirical MSISE00 model, which is based on observational data, suggests a global increase in total atomic oxygen abundance during the equinoxes. However, this increase cannot be explained by a simple redistribution of [O] within the thermosphere, as it represents a global-scale enhancement of atomic oxygen levels. The most plausible mechanism for controlling the global abundance of [O] in the thermosphere is the downward transfer of atomic oxygen via eddy diffusion.

At present, no alternative explanation sufficiently accounts for the global increase in total atomic oxygen during the equinoxes. This phenomenon remains a key area of interest in understanding the aeronomic processes governing thermospheric composition and its impact on ionospheric variability.

 

How to cite: Perrone, L. and Mikhaylov, A.: Equinoctial asymmetry in mid-latitude NmF2 noontime peaks: A formation mechanism , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7057, https://doi.org/10.5194/egusphere-egu26-7057, 2026.

EGU26-7177 | Posters on site | EMRP2.6

Physically constrained empirical modelling of climatological F-region magnetic field and electric current variations 

Gauthier Hulot, Martin Fillion, Patrick Alken, Astrid Maute, and Gary Egbert

The Earth’s ionosphere hosts a complex electric current system that generates magnetic fields. The study of these electric currents and fields provides crucial insights into the ionosphere-thermosphere system, lower atmospheric dynamics, magnetospheric physics, and ionospheric plasma distribution and dynamics.

A particularly valuable dataset to study these currents and fields comes from magnetic measurements acquired by low Earth orbit (LEO) satellites. Some of these satellites provide high-accuracy vector magnetic data that are calibrated using onboard independent scalar measurements. This is the case for the ESA Earth Explorer Swarm satellite constellation, the CHAMP satellite, or the more recently launched MSS-1 satellite. Other satellites, such as the GRACE, GRACE-FO, CryoSat-2, and GOCE satellites, provide complementary, less-accurate platform magnetic vector data, which help improve the overall space-time satellite data coverage. Data from all these satellites are already used to recover and study the signals from the Earth’s outer core, the lithosphere, the oceans, the magnetospheric and the E-region ionospheric currents, as well as the currents induced in the solid Earth by these time-varying ionospheric and magnetospheric fields.

Since LEO satellites orbit within the ionospheric F region, they also provide valuable in situ measurements of F-region ionospheric magnetic fields and electric currents. Interpreting the highly dynamic and spatially complex F-region signals in data from satellites at different altitudes and with very different geographic and local time coverage, however, is a challenging problem. A traditional approach in geomagnetism is to construct empirical models to extract and synthesize signals of interest from multiple data sources. Applied to F-region ionospheric fields and currents, it generally leads to strongly underdetermined inverse problems that can hardly be solved robustly due to incomplete satellite data coverage, even with modern satellite data. Recent research has nevertheless demonstrated that additional progress could be made by relying on optimized spatial basis functions using numerical simulations from realistic physics-based models, such as the Thermosphere-Ionosphere-Electrodynamics General Circulation Model. Such an approach has many advantages, including the ability to fill gaps at altitudes where no satellite data are available and to improve model numerical stability.

We will present our first very encouraging attempt to build a climatological model of F-region magnetic fields and ionospheric currents based on such an approach. Possible avenues for future improvements will also be discussed.

How to cite: Hulot, G., Fillion, M., Alken, P., Maute, A., and Egbert, G.: Physically constrained empirical modelling of climatological F-region magnetic field and electric current variations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7177, https://doi.org/10.5194/egusphere-egu26-7177, 2026.

EGU26-8389 | Orals | EMRP2.6

Status and Latest Results from NASA’s Electrojet Zeeman Imaging Explorer (EZIE)  

Jeng-Hwa Yee, William H. Swartz, Viacheslav Merkin, Rafael Mesquita, Nelofar Mosavi-Hoyer, Rebecca Wind-Kelly, Marc Hoffman, and Sidharth misra and the NASA EZIE Mission Science Team

EZIE, the Electrojet Zeeman Imaging Explorer, is a NASA three-Cubesat Heliophysics mission launch on March, 14, 2025. It employs four downward and cross-track looking miniaturized radiometers on each of the 6U CubeSat, flying in a pearls-on-a-string managed formation, to measure, for the first time, the two-dimensional structure and the temporal evolution of the electrojets flowing at altitudes of ~100–130 km. The four identical radiometers simultaneously measure polarimetric radiances of the molecular oxygen thermal emission at 118 GHz and employs the Zeeman sensing technique to obtain the current-induced magnetic field vectors at ~80 km, an altitude region very close to the electrojet.  This measurement technique allows for the remote sensing of the meso-scale structure of the electrojets at four different cross-track locations simultaneously at altitudes notoriously difficult to measure in situ. Differential drag maneuvers are used to manage satellite along-track temporal separation to within 2–10 minutes between adjacent satellite to record the electrojet temporal evolution without the need for on-board propulsion. The combination of the sensing technique, compact instrument and Cubesat technologies allow EZIE to cost-effectively obtain never-before “mesoscale” measurements needed to understand how the solar wind energies stored in the magnetosphere are transferred to the thermosphere and ionosphere.  In this paper, we will present the current status of the EZIE mission and a summary of the measurement products and its latest results.

How to cite: Yee, J.-H., Swartz, W. H., Merkin, V., Mesquita, R., Mosavi-Hoyer, N., Wind-Kelly, R., Hoffman, M., and misra, S. and the NASA EZIE Mission Science Team: Status and Latest Results from NASA’s Electrojet Zeeman Imaging Explorer (EZIE) , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8389, https://doi.org/10.5194/egusphere-egu26-8389, 2026.

EGU26-10534 | Posters on site | EMRP2.6

Swarm After 12 Years in Orbit: Mission Status, Instrument Performance, and Data Quality 

Enkelejda Qamili, Anja Strømme, Nils Olsen, Roberta Forte, Vincenzo Panebianco, Lars Tøffner-Clausen, Jonas Bregnhøj Nielsen, Stephan Buchert, Christian Siemes, Anna Mizerska, Florian Partous, Elisabetta Iorfida, Lorenzo Trenchi, and Antonio de la Fuenete

Launched by the European Space Agency (ESA) in November 2013, the three-satellite Swarm constellation continues to deliver high-quality measurements of Earth’s magnetic field and the surrounding plasma environment. After more than 12 years in orbit, the mission has achieved remarkable scientific results, deepening our understanding of geomagnetic field dynamics and supporting applications that go well beyond the mission’s original goals.

Equipped with 7 complementary instruments each spacecraft — including a Vector Field and an Absolute Scalar Magnetometer (VFM and ASM); star trackers (STR); a dual-frequency GPS receiver (GPSR); an accelerometer (ACC); an Electric Field Instrument (EFI), composed of two Langmuir Probes (LPs) and two Thermal Ion Imagers (TIIs) — Swarm has become a pivotal reference for geophysical research, supporting advances in areas such as core dynamics, ionospheric and magnetospheric processes, space weather monitoring, and the characterization of electric currents throughout the Geospace environment.

This paper presents a comprehensive overview of the current status of the Swarm mission and constellation, with particular focus on the long-term performance, stability, and calibration of its instruments. The discussion highlights how the constellation’s unique configuration and consistently high data quality have ensured the continuity and reliability of key geophysical observations for more than a decade, with a look at plans for the next future of the mission.

Furthermore, we outline the significant enhancements introduced with the latest Swarm data-processing baseline, which improves the accuracy, consistency, and overall usability of the mission’s data products.

How to cite: Qamili, E., Strømme, A., Olsen, N., Forte, R., Panebianco, V., Tøffner-Clausen, L., Bregnhøj Nielsen, J., Buchert, S., Siemes, C., Mizerska, A., Partous, F., Iorfida, E., Trenchi, L., and de la Fuenete, A.: Swarm After 12 Years in Orbit: Mission Status, Instrument Performance, and Data Quality, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10534, https://doi.org/10.5194/egusphere-egu26-10534, 2026.

EGU26-11045 | Posters on site | EMRP2.6

A World without Low Earth Orbit High-Precision Magnetometry: the next assessment 

Guram Kervalishvili, Maximilian Arthus Schanner, Ingo Michaelis, Monika Korte, Christopher Finlay, Clemens Kloss, Martin Rother, Jan Rauberg, and Enkelejda Qamili

High-precision magnetometry with absolute accuracy is crucial for monitoring the Earth’s magnetic field and advancing our understanding of core, lithospheric, and magnetospheric dynamics. Missions such as Ørsted, CHAMP (CHAllenging Minisatellite Payload), and ESA’s Swarm constellation have demonstrated the unique value of high-precision vector field and scalar magnetometer measurements carried out with absolute accuracy in Low Earth Orbit (LEO). Now imagine a world in which dedicated geomagnetic missions in LEO reach the end of their operational lifetimes, expected or otherwise, with no replacements in place. Without the insights provided by missions like Ørsted, CHAMP, and Swarm, we would lose a critical high-resolution view of Earth’s magnetic environment, leaving many variations unresolved. Moreover, data from dedicated magnetic missions are integral for calibrating platform magnetometers aboard satellites not designed for magnetic measurements. While such instruments remain operational, they lack the precision to capture fine-scale signals. Furthermore, without absolute-accuracy reference measurements, platform magnetometer data become less reliable, leading to increased inconsistencies across datasets.

Here, we examine the consequences of losing high-precision magnetometry with absolute accuracy in LEO for the calibration of platform magnetometers on satellites not dedicated to magnetic measurements. While reference geomagnetic information could still be derived from less accurate sources, such as ground-based observatory networks, these alternatives lack the spatial and temporal resolution uniquely provided by LEO observations and suffer from uneven global coverage, particularly over the oceans and other remote regions where observatories are sparse. Consequently, geomagnetic field models derived from such data would exhibit reduced resolution and accuracy, limiting their reliability and scientific scope. These deficiencies would propagate directly into the calibration of platform magnetometers, degrading their precision and consistency. This cascading effect would significantly impair our ability to monitor, understand, and model the dynamic geomagnetic field, including contributions from the core, lithosphere, and magnetosphere. Maintaining accurate, high-precision magnetometry in LEO is therefore essential to preserve the integrity of geomagnetic science and to support its wide range of scientific and practical applications.

How to cite: Kervalishvili, G., Schanner, M. A., Michaelis, I., Korte, M., Finlay, C., Kloss, C., Rother, M., Rauberg, J., and Qamili, E.: A World without Low Earth Orbit High-Precision Magnetometry: the next assessment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11045, https://doi.org/10.5194/egusphere-egu26-11045, 2026.

EGU26-11506 | ECS | Posters on site | EMRP2.6

Substorm evolution as viewed from a data assimilation technique, Lompe. 

Fasil Kebede, Karl Laundal, Michael Madelaire, and Spencer Hatch

Substorms are transient, explosive events during which energy accumulated in the magnetosphere is rapidly released and dissipated in the high-latitude ionosphere. These events typically last 1–2 hours and may occur several times per day. Despite extensive observational and theoretical efforts, the physical processes governing substorm onset in the magnetosphere and the coupled ionospheric response remain incompletely understood. In particular, the spatiotemporal evolution of electrodynamic parameters during substorms and their dependence on solar wind driving require further investigation.

In this study, we integrate satellite and ground-based observations with the data assimilation technique, Local Mapping of Polar Ionospheric Electrodynamics (Lompe), to examine the global evolution of ionospheric electrodynamics during substorm events. Using Lompe, we reconstruct maps of ionospheric electric potential, ionosphere convection patterns, and field-aligned current systems, and analyze their temporal development throughout substorm phases. These parameters are analyzed in relation to the orientation of the interplanetary magnetic field (IMF). In addition, magnetospheric dynamics during substorms is inferred from estimates of the reconnection electric field, derived by calculating magnetic flux transfer across the open–closed field line boundary.

Our results provide a comprehensive global characterization of the polar ionospheric response to substorms and offer additional insights into the coupling between magnetospheric reconnection processes and ionospheric electrodynamics.

How to cite: Kebede, F., Laundal, K., Madelaire, M., and Hatch, S.: Substorm evolution as viewed from a data assimilation technique, Lompe., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11506, https://doi.org/10.5194/egusphere-egu26-11506, 2026.

EGU26-11552 | Posters on site | EMRP2.6

Swarm Electric Field Instruments, processors and data quality: evolutions, new baseline and scientific highlights 

Roberta Forte, Enkelejda Qamili, Vincenzo Panebianco, Anna Mizerska, Florian Partous, Stephan Buchert, Matthias Förster, Lorenzo Trenchi, Alessandro Maltese, Lars Tøffner-Clausen, Nils Olsen, Anja Stromme, and Antonio De la Fuente

ESA Earth Explorer Swarm mission, launched in November 2013 with the purpose of exploring and understanding the Earth’s interior and its environment, provided significant achievements in the observation of the geomagnetic field, the ionosphere, and electric currents. And it continues contributing to geomagnetism and ionospheric science fields.

Each of the three satellites of the Swarm constellations carries onboard a set of instruments to achieve the mission objectives: a Vector Field and an Absolute Scalar Magnetometer (VFM and ASM); three star trackers (STR) for accurate attitude determination and, recently, for energetic particle detection; a dual-frequency GPS receiver (GPSR); an accelerometer (ACC); an Electric Field Instrument (EFI), composed of two Langmuir Probes (LPs) and two Thermal Ion Imagers (TIIs), dedicated to electric field and plasma measurements. The products derived from EFI instruments represent the focus of this work.

A defining feature of the Swarm mission is its commitment to continuous improvement. Since its launch, advancements in data processing algorithms have been continuously applied: these updates have not only maintained the good quality of Swarm's measurements but have also allowed the mission to evolve and continue meeting the needs of the scientific community. These refinements served the development of novel Swarm-based data products and services, further broadening the mission’s impact, and allowing it to overcome the initial objectives and go beyond its original scope, such as in the Space Weather field.

In December 2025, the most recent baseline has been transferred to operations, delivering updated datasets and evolved products.  These algorithm updates greatly impacted the EFI LP products.  This work will provide an overview of the improvements applied on Swarm plasma data products: detailed analyses are presented, dedicated to new plasma densities and temperatures parameters, new flags, and other upgrades; comparisons with other L1B and L2 Swarm products are performed; case studies in correspondence of recent main Space Weather events are also displayed, to highlight the innovative application of Swarm to this field. 

How to cite: Forte, R., Qamili, E., Panebianco, V., Mizerska, A., Partous, F., Buchert, S., Förster, M., Trenchi, L., Maltese, A., Tøffner-Clausen, L., Olsen, N., Stromme, A., and De la Fuente, A.: Swarm Electric Field Instruments, processors and data quality: evolutions, new baseline and scientific highlights, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11552, https://doi.org/10.5194/egusphere-egu26-11552, 2026.

EGU26-11971 | Posters on site | EMRP2.6

Swarm Investigation of Space Weather and Natural Hazards Effects 

Georgios Balasis, Ewa Slominska, Octav Marghitu, Constantinos Papadimitriou, Adamantia Zoe Boutsi, Adrian Blagau, Omiros Giannakis, and Elisabetta Iorfida

Swarm Investigation of SpAce Weather and NAtural HazaRds Effects (Swarm-AWARE) is a new European Space Agency (ESA) project funded by the Earth Observation (EO) Science for Society programme. The main goal of the Swarm-AWARE project is to apply innovative techniques and deliver new scientific discoveries of the Earth system, pertinent to space weather (SWE) and natural hazards (NH) effects. Relevant achievements are expected through a systematic investigation of Swarm-derived indices related to magnetospheric substorm activity, field-aligned currents (FACs), magnetic storm activity, ultra-low frequency (ULF) plasma waves and equatorial Spread-F (ESF) events (plasma bubbles). Both the SWE and NH scientific targets have great societal impacts, since SWE effects can include damage and disruption to power distribution networks on the ground, while NH can result in a broad range of effects, from various perturbations of the ionosphere and related disruptions of, e.g., positioning (GPS, GNSS, Galileo) or telecommunication services (notably affected also by strong SWE events), up to most severe consequences, including the loss of human lives.

We tackle this great challenge through the use of state-of-the-art machine learning (ML) and advanced time series analysis (TSA) techniques. The Swarm-AWARE project exploits the unique capabilities of the Swarm mission data, including multi-point observations, together, significantly, with complementary ground data (e.g., SuperMAG magnetometer network and all-sky cameras). Furthermore, in addition to exploiting the unique nature of these combined data sets, Swarm-AWARE highlights potential new foci for future Swarm scientific studies. This research also investigates concepts for potentially new Swarm data products, which address the challenges associated with the impact of geological hazards (e.g., earthquakes, volcanic eruptions) at middle to low latitudes. In parallel, by providing longer time series of the Swarm-derived SFAC index, together with Swarm AE-like and Swarm SYM-H-like geomagnetic activity indices, that currently exist, Swarm-AWARE helps to shed new light on the North-South ionospheric asymmetry, in particular at high latitudes.

How to cite: Balasis, G., Slominska, E., Marghitu, O., Papadimitriou, C., Boutsi, A. Z., Blagau, A., Giannakis, O., and Iorfida, E.: Swarm Investigation of Space Weather and Natural Hazards Effects, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11971, https://doi.org/10.5194/egusphere-egu26-11971, 2026.

EGU26-12104 | ECS | Posters on site | EMRP2.6

Multi-scale Reconstruction of Field-Aligned Currents Using the Swarm Spacecraft 

Rafal Gajewski and Ravindra Desai

Field-aligned currents (FACs) are a primary channel for the transport of energy and momentum from the magnetosphere into the ionosphere, where they strongly influence atmospheric dynamics through Joule heating. Due to significant spatial and temporal variability, accurately determining FAC density vectors from magnetic field measurements remains challenging. Amongst available techniques, the curlometer method applied to multi-spacecraft magnetic field observations provides the most reliable means of estimating current density. A full three-dimensional reconstruction requires magnetic field measurements at four distinct locations arranged in a near-regular tetrahedral configuration. In contrast, configurations involving fewer spacecraft may be employed, though this approach relies on the assumption of magnetic field stationarity and favourable spacecraft alignment. Here, we investigate current density reconstruction from Swarm magnetic field measurements and evaluate associated quality metrics for a range of conditions for scenarios, spanning macro-, meso-, and micro-scale FAC structures during geomagnetic storms. We then apply this method to simulated trajectories of the tetrahedral configuration proposed for the ROARS F3 mission concept, quantifying the improvements in FAC estimation enabled by a dedicated four-spacecraft mission to Low Earth Orbit.

How to cite: Gajewski, R. and Desai, R.: Multi-scale Reconstruction of Field-Aligned Currents Using the Swarm Spacecraft, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12104, https://doi.org/10.5194/egusphere-egu26-12104, 2026.

EGU26-13266 | ECS | Orals | EMRP2.6

ROARS: Research Observatory for Atmospheric Responses to Sun-magnetosphere interactions 

James Blake, Ravindra Desai, Stas Barabash, Johnathan Burchill, Matthew Brown, John Coxon, Thomas Daggitt, Malcolm Dunlop, Rico Fausch, Bogdan Hnat, Gauthier Hulot, Jean-Michel Leger, Dong Lin, Rumi Nakamura, Hans Nilsson, Evgeny Panov, Shreedevi Radhakrishna, Audrey Vorburger, Maria Walach, and Xiao-Dong Wang

The Earth’s upper atmosphere is highly sensitive to solar activity and the solar wind-magnetosphere interaction. Magnetospheric current systems close through the ionosphere, where ion-neutral collisions and enhanced energetic particle precipitation can significantly modulate the spatial and temporal variability of the atmosphere's outer extent. Unlike the many isolated in-situ measurements conducted by previous space missions, distributed observations of neutral particles, plasma, and magnetic fields by a tetrahedron of micro-satellites, combined with precise tracking of satellite orbital dynamics, provide the global perspective needed to disentangle the complex transfers of energy and momentum through the tightly coupled magnetosphere-ionosphere-thermosphere system.

In this presentation, we outline the ROARS F3 mission architecture. This mission seeks to obtain the first full curlometer magnetic field and energetic particle precipitation measurements in low Earth orbit (LEO), alongside concurrent measurements of the ambient plasma and neutral populations across a range of altitudes, latitudes, and longitudes. The measurement strategy is designed to resolve and characterise the energy and momentum entering the upper atmosphere, the multi-scale pathways through which these are redistributed, and the feedback mechanisms coupling back to the broader geospace environment. A comprehensive ground segment will simultaneously provide context by relating information on D- and E-region dynamics to the in-situ measurements.

How to cite: Blake, J., Desai, R., Barabash, S., Burchill, J., Brown, M., Coxon, J., Daggitt, T., Dunlop, M., Fausch, R., Hnat, B., Hulot, G., Leger, J.-M., Lin, D., Nakamura, R., Nilsson, H., Panov, E., Radhakrishna, S., Vorburger, A., Walach, M., and Wang, X.-D.: ROARS: Research Observatory for Atmospheric Responses to Sun-magnetosphere interactions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13266, https://doi.org/10.5194/egusphere-egu26-13266, 2026.

EGU26-13271 | Posters on site | EMRP2.6

Innovative Measurements of Auroral Geophysics for Education and Research (IMAGER) 

Johnathan Burchill, Kaleigh Beer, Victor Borges, Ravindra Desai, Mykola Ivchenko, David Knudsen, Chase Rupprecht, Theodoros Sarris, and Emma Spanswick

This presentation provides an overview and update on the Canadian Space Agency sponsored IMAGER project, which has two main objectives: 1) Fly an upgraded ionospheric ion analyzer (the 'MPI') on the CalgaryToSpace FrontierSat cubesat to characterize ionospheric flows in the vicinity of the aurora and STEVE and investigate satellite charging; 2) Develop and fly an improved analyzer to measure ionospheric ion drift as part of the Swedish SYSTER suborbital rocket mission to investigate ionosphere-thermosphere coupling. The design, development, integration and test activities are conducted by students in the spirit of the training component of CSA's Flights and Fieldwork for the Advancement of Science and Technology (FAST) programme. FrontierSat and SYSTER are scheduled for launches in 2026. We introduce each mission's scientific rationale, highlight recent technical and training developments, and briefly describe several potential future mission opportunities in upper-atmospheric cold-plasma physics.

How to cite: Burchill, J., Beer, K., Borges, V., Desai, R., Ivchenko, M., Knudsen, D., Rupprecht, C., Sarris, T., and Spanswick, E.: Innovative Measurements of Auroral Geophysics for Education and Research (IMAGER), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13271, https://doi.org/10.5194/egusphere-egu26-13271, 2026.

EGU26-13435 | Posters on site | EMRP2.6

ESA's VirES for Swarm service in 2026 

Martin Pačes and Ashley Smith

The VirES service launched publicly in 2016 and has continuously evolved, adding more datasets and features every year [1]. It comprises four main components: server, web client, Python client, and JupyterHub, providing a range of routes to access, visualise, and process the Swarm product portfolio [2] and more.

Notable features include:
- LEO magnetometry from other missions: CHAMP, CryoSat-2, GRACE, GRACE-FO, GOCE
- INTERMAGNET ground observatories
- Notebook-based cookbook [3]
- Heliophysics API (HAPI) [4]

Building upon robust data access via VirES and HAPI, Swarm DISC (Swarm Data, Innovation, and Science Cluster) is also developing the SwarmPAL Python package [5] to facilitate higher-level analysis. Overall, we aim to produce a sustainable ecosystem of tools and services, which together support accessibility, interoperability, open science, and cloud-based processing [6]. All services are available freely to all, and the software is developed openly on GitHub [7,8].

The work presented is the result of many partners across Swarm DISC.
[1] https://vires.services/changelog
[2] https://swarmhandbook.earth.esa.int
[3] https://notebooks.vires.services
[4] https://vires.services/hapi
[5] https://swarmpal.readthedocs.io
[6] https://doi.org/10.3389/fspas.2022.1002697
[7] https://github.com/ESA-VirES
[8] https://github.com/Swarm-DISC

How to cite: Pačes, M. and Smith, A.: ESA's VirES for Swarm service in 2026, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13435, https://doi.org/10.5194/egusphere-egu26-13435, 2026.

EGU26-15926 | Orals | EMRP2.6

Investigating Space Radiation and Atmospheric Climate Impacts with the Canadian RADICALS Mission 

Ian Mann, Chris Cully, Robert Fedosejevs, Steven Knudsen, David Milling, Greg Enno, Michael Lipsett, Robert Zee, Robert Rankin, Martin Connors, Kathryn McWilliams, William Ward, Robyn Fiori, Leonid Olifer, Louis Ozeke, Robert Marshall, David Cullen, David Barona, Andrew Howarth, and Andrew Yau

This presentation provides an overview of the latest designs and development of the RADiation Impacts on Climate and Atmospheric Loss Satellite (RADICALS) mission, and which will launch in October 2027. The RADICALS is a Canadian small satellite mission with a payload designed to characterise energetic particle precipitation (EPP), to assess the physical mechanisms which cause it, and investigate the related impacts on the Earth’s atmosphere. EPP plays a critical role in altering atmospheric chemistry, particularly through the production of NOx and HOx, which catalytically destroy ozone in the middle atmosphere. The RADICALS will focus on measuring the energy input from precipitating energetic particles into the atmosphere, shedding new light on the connection between space weather and climate. Operating in a polar orbit, the RADICALS payload contains dual High Energy Particle Telescope (HEPT) suites (each comprising high and low energy telescopes, and a high temporal resolution scintillator), and dual X-Ray Imager (XRI) suites. When mounted on the spinning RADICALS spacecraft they will provide pitch angle distributions of trapped radiation belt electrons and solar energetic protons, twice per spin, as well as the associated Bremsstrahlung X-rays from atmospheric interactions. The mission's unique back-to-back HEPT suite design will measure both down-going and up-going particles simultaneously, while the XRI will remotely sense particle precipitation via X-ray emissions as well as monitoring lower energy electrons as a secondary product. The payload also includes a pair of boom-mounted fluxgate magnetometers and a 3-axis and search coil magnetometer to substantiate particle measurements with the local magnetic wave activity. By resolving the electron loss cone and quantifying the energy flux of precipitating particles, RADICALS will provide essential data for understanding how space radiation influences atmospheric chemistry, particularly during geomagnetic storms.

How to cite: Mann, I., Cully, C., Fedosejevs, R., Knudsen, S., Milling, D., Enno, G., Lipsett, M., Zee, R., Rankin, R., Connors, M., McWilliams, K., Ward, W., Fiori, R., Olifer, L., Ozeke, L., Marshall, R., Cullen, D., Barona, D., Howarth, A., and Yau, A.: Investigating Space Radiation and Atmospheric Climate Impacts with the Canadian RADICALS Mission, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15926, https://doi.org/10.5194/egusphere-egu26-15926, 2026.

EGU26-17072 | Orals | EMRP2.6

Compressional Pc3-4 magnetic pulsations in the topside ionosphere: observations from multiple LEO satellites 

Chao Xiong, Hermann Luehr, Chunyu Xu, and Haibin Liu

Pc3-4 magnetic pulsations within the 16-100 mHz frequency range are mainly driven by the upstream waves (UWs) in the Earth’s foreshock region, which serves as a critical link for transferring energy from the solar wind into the magnetosphere-ionosphere system. High-precision magnetometer data from low Earth orbit (LEO) satellites, like CHAMP, Swarm and MSS-1, covering two solar cycles (from 2001-2025), provide a good database for resolving the characteristics of UWs. In this report, we performed a comprehensive analysis on UWs in the topside ionosphere, including their dependences on solar wind and interplanetary magnetic field conditions, season, magnetic local time, as well as latitude and longitudes. In addition, by analyzing the simultaneously measurements from these satellites with certain spatial separation, the propagation of UWs in the topside ionosphere has also been discussed.

How to cite: Xiong, C., Luehr, H., Xu, C., and Liu, H.: Compressional Pc3-4 magnetic pulsations in the topside ionosphere: observations from multiple LEO satellites, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17072, https://doi.org/10.5194/egusphere-egu26-17072, 2026.

EGU26-17103 | Posters on site | EMRP2.6

Low-latitude effects of high-latitude field-aligned currents 

Karl M. Laundal, Andreas Skeidsvoll, Beatrice Braileanu, Spencer Hatch, Nils Olsen, Colin Waters, Michael Madelaire, Fasil Kebede, Chris Finlay, Clemens Kloss, and Jesper Gjerloev

High-latitude field-aligned currents (FACs) reflect, in steady-state, the force balance between magnetospheric plasma dynamics and the collisional coupling of plasma to the neutral atmosphere in the ionosphere. Assessing the impact of high-latitude FACs at low latitudes is difficult for at least two reasons. First, FACs are primarily inferred from magnetometer measurements in low-Earth orbit by estimating the radial current using horizontal magnetic field perturbations and converting it to a FAC using a geometric factor. While this yields a locally correct estimate of the FAC density, the magnetic field generated by a radial current system differs from that generated by the corresponding FAC system when field lines are not radial. As a result, the magnetic field of the horizontal component of FACs, including their remote magnetic field observed at low latitudes, are neglected. Second, in many numerical simulations, FACs are coupled to the ionosphere only at high latitudes, while boundary conditions are imposed at lower latitudes, arguably making it difficult, from a fundamental physics perspective, to trace how high-latitude forcing influences low latitudes.
Here we use AMPERE estimates of high-latitude FACs at 10-min resolution derived from magnetometer measurements on the Iridium satellite constellation to quantify their low-latitude impact. FACs in both polar regions are used to calculate the remote magnetic field using the integration method of Engels and Olsen (1998, https://doi.org/10.1016/S1364-6826(98)00094-7). A recently developed magnetosphere-ionosphere coupling model (Laundal et al. 2025, https://doi.org/10.5194/angeo-43-803-2025) is used to compute the associated penetration electric field. The resulting magnetic and electric fields are compared with observations at low latitudes.

How to cite: Laundal, K. M., Skeidsvoll, A., Braileanu, B., Hatch, S., Olsen, N., Waters, C., Madelaire, M., Kebede, F., Finlay, C., Kloss, C., and Gjerloev, J.: Low-latitude effects of high-latitude field-aligned currents, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17103, https://doi.org/10.5194/egusphere-egu26-17103, 2026.

EGU26-18081 | ECS | Posters on site | EMRP2.6

New developments of the CHAOS ionospheric field model 

Clemens Kloss and Nikolaj Schejbel Nielsen

The CHAOS-8 geomagnetic field model series describes the time-dependent near-Earth geomagnetic field under quiet conditions since 1999. It is derived from magnetic field observations from low-Earth orbit satellites, such as Swarm, CHAMP, MSS-1, and CSES, as well as annual differences of revised monthly means of ground observatory measurements. Starting with the 8th generation, the series co-estimates a climatological model of the ionospheric E-layer currents with a focus on accounting for their magnetic signals in the polar regions, which can be significant even under quiet and dark conditions. This model follows the AMPS approach (Laundal et al., 2018), utilizing magnetic apex coordinates and magnetic local time to describe large-scale patterns efficiently. Additionally, it uses multiple external parameters, including the Interplanetary Magnetic Field, dipole tilt angle, and magnetosphere-ionosphere coupling functions, to represent variability on seasonal, daily, and shorter time scales.

Although the CHAOS ionospheric field model can successfully represent the average patterns in the polar ionospheric E-layer field, limitations remain. Most notably, it is less suitable at non-polar latitudes, where the Sq current system dominates, because it lacks longitude dependence. Moreover, the reliance on simple dependencies on external parameters to capture temporal variability may be overly restrictive, particularly for seasonal and long-term changes. Finally, since the CHAOS ionospheric field is estimated only from satellite data, both the internal and ionospheric contributions are treated as internal sources.

This work presents ongoing efforts to address limitations in the CHAOS ionospheric field. Test models are estimated from satellite data using monthly and shorter time windows to capture seasonal variability better. Longitudinal dependence is introduced to provide a more accurate representation of the field at low latitudes, following the approach of the comprehensive model (Sabaka et al. 2003), while continuing to rely on apex coordinate systems. By comparing model predictions to ground observatory data, the potential of incorporating observatory measurements into the model estimation is explored to enhance the separation of internal and ionospheric contributions.

How to cite: Kloss, C. and Schejbel Nielsen, N.: New developments of the CHAOS ionospheric field model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18081, https://doi.org/10.5194/egusphere-egu26-18081, 2026.

EGU26-18301 | ECS | Posters on site | EMRP2.6

Identification of the principal characteristics of an ionospheric Langmuir Probe for furture satellite space mission 

Giulio La Rovere, Piero Diego, and Mirko Piersanti

Langmuir probes are instruments devoted to the in-situ measurement of plasma parameters,
such as floating and plasma potentials, as well as density and electrons temperature. Un
derstanding the interactions among this type of payload, the satellite body, and the orbital
environment is crucial to determine whether specific geometries and conditions could create
phenomena that may affect the plasma measurement. A realistic CAD model of an ionospheric
plasma probe is implemented with the SPIS (Spacecraft Plasma Interaction Software) program
ming environment. SPIS, developed by the SPINE community, is used to simulate the mutual
interaction between the satellite and the probe with the ionospheric plasma (LEO) using the
particle-in-cell method. The results of the numerical simulation are then compared with real
satellite data (from Swarm, CSES, and DEMETER missions) and data collected from a similar
instrument of the INAF-IAPS diagnostic system of the INAF-IAPS Plasma Chamber in Rome

How to cite: La Rovere, G., Diego, P., and Piersanti, M.: Identification of the principal characteristics of an ionospheric Langmuir Probe for furture satellite space mission, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18301, https://doi.org/10.5194/egusphere-egu26-18301, 2026.

EGU26-19387 | Orals | EMRP2.6

Advanced Modelling of Geospace (AMOG) Using Satellite Platform Magnetometers 

Nils Olsen, Fabrice Cipriani, Elisabetta Iorfida, Per Lundahl Thomsen, and Flemming Hansen

Continuous monitoring of electric current systems in Earth’s environment, including the ionosphere and magnetosphere, is essential for characterising geospace. Such observations are required, for example, to determine the energy input into the upper atmosphere and to monitor disturbances in the space environment and associated hazards. This monitoring can be achieved through magnetic field measurements acquired both on the ground and in space.

The spatio-temporal sampling provided by dedicated magnetic satellite missions such as Swarm and MSS can be significantly enhanced by incorporating platform magnetometer data from non-dedicated missions, including CryoSat-2, GRACE, and GRACE-FO.

This presentation reports recent achievements in the use of platform magnetometer data within a study funded by ESA’s General Support Technology Programme (GSTP). In particular, it highlights the calibration and provision of magnetic field data from ESA’s Aeolus satellite.

How to cite: Olsen, N., Cipriani, F., Iorfida, E., Thomsen, P. L., and Hansen, F.: Advanced Modelling of Geospace (AMOG) Using Satellite Platform Magnetometers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19387, https://doi.org/10.5194/egusphere-egu26-19387, 2026.

EGU26-19482 | Posters on site | EMRP2.6

Development of a Solid-State Detector for Use in Ionospheric Environments 

Chih-Yu Chiang, Tzu-Fang Chang, Yu-Rong Cheng, Tzu-En Yen, Sheng-Cheng Tsai, Cheng-Tien Chen, Ping-Ju Liu, and Yung-Tsung Cheng

Solid-state detectors (SSDs) are commonly used in space environments to detect particles and radiation. The Multiple Particle Analyzer (MPA) is a scientific payload built upon an SSD application. The MPA will be carried on the Formosat-8C satellite (FS-8C) in the future to monitor global ionospheric space weather. Its design was originally derived from the STE (Supra Thermal Electron) detector on the STEREO satellite. This analyzer utilizes a multi-channel detector component that can measure electrons, ions, and neutral atoms in the energy range of approximately 1 to 200 keV. The team from National Cheng Kung University (NCKU) is currently developing and testing the scientific payload, with a flight model of the MPA expected to be submitted in the fourth quarter of 2026. The FS-8C satellite is scheduled to launch at the end of 2027.

How to cite: Chiang, C.-Y., Chang, T.-F., Cheng, Y.-R., Yen, T.-E., Tsai, S.-C., Chen, C.-T., Liu, P.-J., and Cheng, Y.-T.: Development of a Solid-State Detector for Use in Ionospheric Environments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19482, https://doi.org/10.5194/egusphere-egu26-19482, 2026.

A recent update of the MCM series of magnetic field models and associated core surface flows is presented. The models were derived sequentially from year 1999 to 2025, using magnetic satellite and ground observatory data. A linear Kalman filter approach and prior statistics based on numerical dynamo runs were used. The core field, the secular variation and the core surface flow models present the same characteristics as previous versions up to 2023 and we investigate how this behaviour evolves over the most recent years. In particular, before 2023 filtering out the flow variation periods longer than ∼11.5 years revealed filtered azimuthal flow with ∼7 years periodicities and patterns propagating westward by ∼60deg longitude per year. Preliminary results show that the same patterns are maintain over the most recent epochs.

How to cite: Lesur, V.: Core magnetic field and associated surface flow variations from 1999 to 2025, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22028, https://doi.org/10.5194/egusphere-egu26-22028, 2026.

EGU26-288 | Posters on site | EMRP2.8

Integrated Geophysical Studies for tracing the Northern Extension of the Subsurface Spillway Fault, Aswan, Egypt 

Ahmed Khalil, Ahmed El Emam, Ahmed Hamed, Mohamed Khalifa, and Abdou Khalaf

The main object of this study is to trace the northern extension of the subsurface Spillway fault, Aswan, Egypt. To achieve this, we used two geophysical techniques, magnetic and passive seismic surface wave. Magnetic data provides insights into subsurface structures, basement depth and structural trends. While passive seismic surface wave technique (frequency-wavenumber) uses seismic surface waves (Rayleigh wave) to map the subsurface allowing for the evaluation the fault depth. This method relies on data collected from a sensor array that captures wave field information in order to obtain shear wave velocity models. In the current study, 10 microtremor arrays have been conducted north of Ben Ban solar plant location (north of Aswan city), in order to construct 2D profile for tracing the subsurface faults. The obtained results show graben fault, in which areas has low shear wave velocity value (350 m/s) confined between high shear wave velocity (1100 m/s) areas. Also, a detailed land magnetic survey has been carried out for the total component of the geomagnetic field using two overhauser magnetometers. The necessary corrections concerning daily variation, the regional gradient and time variations have been applied. Then, the total magnetic intensity anomaly map (TMI) has been constructed and transformed to the reduced to the pole magnetic map (RTP). The reduction-to-pole magnetic anomaly maps was used to obtain regional extensions of this subsurface structure. Regional–residual separation is carried out using the power spectrum. Also, Edge detection techniques are applied to delineate the structure and hidden anomalies various edge detection techniques including the tilt angle derivative, its total horizontal derivative, and 3D-Euler Deconvolution are applied to delineate the boundaries of these sources. The Euler solutions were superimposed on the tilt angle derivative map, revealing a strong correlation between the techniques, confirming their effectiveness in mapping the area's structural framework. The analysis indicates that the study area is influenced by multiple structural trends. Depth estimation was conducted using multiple approaches, yielding consistent results. The derived depths to the top of basement sources range from 300 to approximately 2500 meters. We can conclude that the obtained graben fault could be considered as an extension of the spillway fault

KEYWORDS
Land magnetic, frequency-wavenumber, Spillway fault, Euler Deconvolution, Edge detection and Spectral analysis.

How to cite: Khalil, A., El Emam, A., Hamed, A., Khalifa, M., and Khalaf, A.: Integrated Geophysical Studies for tracing the Northern Extension of the Subsurface Spillway Fault, Aswan, Egypt, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-288, https://doi.org/10.5194/egusphere-egu26-288, 2026.

EGU26-1241 | ECS | Posters on site | EMRP2.8

New Paleomagnetic Data from South America and Implications for the Southern Hemisphere Geomagnetic Field Evolution 

Sebastian Aguilar Moncada, Gelvam André Hartmann, Wellington P. Oliveira, Andrew J. Biggin, Ricardo Trinidade, Natalia G. Pasqualon, Daniel A. Coppi, Gustavo S. da Silva, Jairo F. Savian, Evandro F. Lima, Fernando R. da Luz, Giovanny Nova, Mauricio Parra, Carlos A. Sommer, Alejandro D. Báez, Alberto T. Caselli, Daniel R. Franco, and Felipe Terra-Nova

The Earth’s magnetic field (EMF), generated by geodynamo processes, varies across multiple timescales ranging from years to billions of years. Integrated analyses of paleodirectional and paleointensity data over the past 10 million years reveal persistent non-dipolar features in the Southern Hemisphere, linked to the South Atlantic Magnetic Anomaly (SAA). However, the spatial and temporal coverage of high-quality paleomagnetic data remains uneven and is particularly scarce in South America. To address this gap, we provide new paleodirections and paleointensities from different volcanic units in Argentina, Colombia and Brazil. New paleodirectional data were obtained from 23 sites of the Auca Mahuida Volcano (0.19-1.53 My; Argentina) by thermal and alternating field demagnetisation protocols. Paleointensity data were obtained from 41 sites in Colombia, Brazil, and Argentina, ranging in age between 0.005-1.95 My using multiple experimental methods, including Triaxe, Wilson, Thermal Thellier, Microwave Thellier, and the Double Heating Technique of Shaw (DHT-Shaw). 

The magnetic mineralogy of the studied volcanic rocks comprises dominantly low-Ti titanomagnetite, as indicated by thermomagnetic curves with susceptibility drop between 550 °C and 580 °C and IRM curves with saturation fields below 300 mT. FORC analyses and Day diagrams reveal the dominance of the Pseudo Single Domain (PSD) state of the magnetic grains. Directional data for the Auca Mahuida Volcano yielded a mean direction (D =356.4°, I = -52.04° and α95 = 6.4°; N = 14; K>50; Vandamme cutoff) that is statistically indistinguishable from the expected direction for a geocentric axial dipole (GAD) field (IGAD = −57.0°) in that location, within the 95% confidence limits. The corresponding VGP dispersion Sb =12.799.3°15.9° agrees well with other studies carried out in the Southern Hemisphere and Paleosecular Variation (PSV) models.

Out of 332 specimens analysed in paleointensity experiments, approximately 20% met our selection quality criteria (f>0.3, n>4, 𝛽<0.1, MADANC<15, DRAT<10, CDRAT<15). Virtual Dipole Moments (VDMs) ranged from 2.45× 10²² Am² to 8.02× 10²² Am² (8 sites in Argentina), 1.64× 10²² Am² to 9.29× 10²² Am² (5 sites in Colombia), and 5.17× 10²² Am² to 5.49× 10²² Am² (2 sites, in Brazil). Most of the normal and reversed sites exhibit paleointensity values within the 95% confidence limits of the geomagnetic field predicted in models such as PADM2M and MCADAM 1b, with two exceptions (Argentina) in 0.34 My and 1.36 My showing values of 3.6× 10²² Am² and 1.19× 10²² Am², respectively, while transitional data display significantly lower intensities  (e.g., 2.45× 10²² Am²).The dispersion (Sb) of the VGPs using alternative selection criteria shows higher values in the analysed sites compared with the expected values for the Southern Hemisphere, deviating from regional PSV models. The variability in paeointensity values, sometimes lower than those predicted by the consulted models, may be related to the presence of the SAA. Further studies and data will be required. The new Paleomagnetic data from various volcanic bodies in South America will contribute to expanding the database for the last 10 Million Years, thereby enhancing the model's accuracy and providing better constraints on its boundary conditions.

How to cite: Aguilar Moncada, S., Hartmann, G. A., Oliveira, W. P., Biggin, A. J., Trinidade, R., Pasqualon, N. G., Coppi, D. A., da Silva, G. S., Savian, J. F., Lima, E. F., da Luz, F. R., Nova, G., Parra, M., Sommer, C. A., Báez, A. D., Caselli, A. T., Franco, D. R., and Terra-Nova, F.: New Paleomagnetic Data from South America and Implications for the Southern Hemisphere Geomagnetic Field Evolution, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1241, https://doi.org/10.5194/egusphere-egu26-1241, 2026.

EGU26-2059 | ECS | Posters on site | EMRP2.8

Does sedimentary facies transformation modulate the recording of orbital forcing? Insights from environmental magnetism and multi-proxy data in the Songnen Basin (NE China) 

Zihan Gao, Zhixiang Wang, Mengmeng Cao, Hongxing Hou, Bingzhang Ren, Ze Zhang, and Rui Zhang

The question of which orbital parameters (eccentricity, obliquity, and precession) drove Pleistocene variability in East Asian monsoon precipitation has become one of the enduring problems in paleoclimatology, yet a consensus remains elusive. Here, we test whether major sedimentary facies transformations can modify the orbital imprint preserved in climate archives by integrating environmental magnetic and non-magnetic proxies from a 954 kyr borehole (47°25′42″N, 125°55′00″E) in the Songnen Basin, NE China. We analyze magnetic susceptibility together with elemental contents and grain-size indices across intervals characterized by pronounced facies transitions. The χlf, χfd, Mn/Fe, Rb/Sr, Fe content, and the percentage of >32 μm (%) show significant correlations with lithological transitions over time. The shift from swamp/peat to lacustrine facies is marked by a notable decline in χlf, Rb/Sr, and Fe flux, while χfd, Mn/Fe, and the percentage of >32 μm (%) exhibit a clear increase. The transition from lacustrine to marginal lacustrine facies shows relatively minor but still distinct changes, with χfd, Mn/Fe, Fe flux, and the percentage of >32 μm (%) increasing significantly. The most pronounced transition occurs around 200 ka, changing aqueous to eolian deposition. During this period, χlf, χfd, and Mn/Fe rise sharply, the Rb/Sr ratio continues to decline, and Fe flux and the percentage of >32 μm (%) display a stable trend with weaker amplitude fluctuations compared to before 200 ka. Spectral and evolutionary spectral analyses show that the dominant orbital periodicity is consistently expressed across facies changes, indicating that facies transformation does not fundamentally reorganize the primary orbital pacing recorded in this sequence. In contrast, the relative power and temporal stability of specific orbital bands vary among proxies, implying proxy-dependent sensitivity rather than archive-dependent forcing. We attribute these differences to differential responses of regional climate components (i.e., temperature, effective moisture, and lake-level variability) to orbital forcing, which in turn regulate magnetic mineral concentration and grain size, detrital input, and chemical transport pathways. Our results highlight that discrepancies among orbital-forcing reconstructions of East Asian rainfall arise mainly from how individual proxies encode climate conditions, rather than from changes in the geological archive itself.

How to cite: Gao, Z., Wang, Z., Cao, M., Hou, H., Ren, B., Zhang, Z., and Zhang, R.: Does sedimentary facies transformation modulate the recording of orbital forcing? Insights from environmental magnetism and multi-proxy data in the Songnen Basin (NE China), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2059, https://doi.org/10.5194/egusphere-egu26-2059, 2026.

EGU26-3369 | Posters on site | EMRP2.8

Magnetostratigraphic dating of the Pulu mammalian fauna in the Nihewan Basin, North China 

Ping Liu, Jiahao Li, and Xianli Gao

Nihewan Basin is one of a series of well-developed East Asian Cenozoic basins in Hebei Province, North China, which are rich sources of mammalian faunas and Paleolithic sites. During the past decades, detailed magnetostratigraphic dating was conducted on the Nihewan Formation and associated mammalian faunas and Paleolithic sites, and the results have contributed significantly to our understanding of the chronostratigraphy of the Nihewan Basin.

The Pulu fauna, one of the Nihewan faunas (sensu lato), is located on the eastern bank of the Huliu River in the Nihewan Basin and contains mammalian fauna in the late Pliocene to early Pleistocene. Here, we selected the fluvio-lacustrine deposits containing the Pulu mammalian fauna to conduct detailed rock magnetic and high-resolution magnetostratigraphy studies, combined with biostratigraphic and lithostratigraphic results, to precisely constraint on the Pulu mammalian fauna. In this study, 466 oriented samples were collected from the fluvio-lacustrine sequences of Pulu section (thickness 112 m) for detailed rock magnetic and magnetic fabric studies. The results showed that the magnetic minerals in the fluvio-lacustrine deposits of the Pulu section are mainly magnetite, maghemite and hematite, with predominantly pseudo-single domain. The Pulu fluvio-lacustrine deposits recorded the early Brunhes normal chron, the Matuyama reverse chron, the Gauss normal chron and the late Gilbert reverse chron. The Pulu mammalian fauna was found during the pre-Réunion Matuyama chron and the post-Kaena Gauss chron with the age about 3.0-2.2 Ma. This study has extended the lower age of the Nihewan faunas to about 3.0 Ma. Furthermore, the paleoclimatic and paleoenvironmental studies in the Nihewan Basin suggested that the evolutionary direction of the Nihewan faunas were influenced by changes in climate and environment during the Pliocene and Pleistocene transitions, and Nihewan faunas evolved towards adapting to a cold and arid environment.

How to cite: Liu, P., Li, J., and Gao, X.: Magnetostratigraphic dating of the Pulu mammalian fauna in the Nihewan Basin, North China, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3369, https://doi.org/10.5194/egusphere-egu26-3369, 2026.

The core function of a marine geomagnetic diurnal variation observatory is to continuously collect geomagnetic diurnal variation data at a fixed ocean depth, and the quality of such data directly determines the accuracy of marine magnetic survey results. In the absence of this data, marine magnetic data cannot be precisely corrected, which in turn leads to significant errors in data processing and ultimately impairs the reliability of magnetic exploration outcomes.

At present, the Sentinel series geomagnetic diurnal variation observatories based on the Overhauser principle are widely adopted in China's marine magnetic survey sector. This paper presents a novel marine geomagnetic testing system developed on the basis of proton precession magnetometers, which offers three key advantages: first, it fills the domestic gap in independently developed products for marine geomagnetic diurnal variation observatories; second, it is designed with 6,000-meter ocean-specific glass floats, making it suitable for deep-sea deployment requirements; third, it achieves substantial improvements in both instrument performance and operational stability. The findings of this study provide an important reference for the technological iteration and application expansion of marine geomagnetic diurnal variation observatories.

How to cite: Chang, W.: Development and Application of Proton Magnetometers in Marine Geomagnetic Diurnal Variation Observatories, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3720, https://doi.org/10.5194/egusphere-egu26-3720, 2026.

EGU26-6673 | Orals | EMRP2.8

Mantle heterogeneities induce time- and space-varying magmatism at the migrating ultraslow Southwest Indian Ridge 

Fei Zhou, Jérôme Dyment, Ingo Grevemeyer, and Chuanzhou Liu

The link between mantle heterogeneity as depicted by geochemical and seismic studies and the magmatism emplaced on the divergent plates remains elusive. Here, we derive variations of magmatism from marine magnetic data and trace mantle heterogeneities beneath the eastern Southwest Indian Ridge over 27 Ma. Three states of magmatism, robust, intermediate, and starved, are identified from the amplitude of magnetic anomalies. Comparing the distribution of magmatism on orthogonal and oblique ridge sections supports an asthenospheric source, not moving with the plates and ridge, as the predominant source of magmatic variations. These variations are therefore linked to different amounts of fertile and refractory mantle in the asthenosphere sampled by the ultraslow spreading center. In the study area, fertile mantle heterogeneities are 10 to 60 km-wide with the ridge migrating at 5 km/Myr in a N30°E direction. This study offers a new approach to constrain deep mantle heterogeneities from shallow crustal observations.

How to cite: Zhou, F., Dyment, J., Grevemeyer, I., and Liu, C.: Mantle heterogeneities induce time- and space-varying magmatism at the migrating ultraslow Southwest Indian Ridge, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6673, https://doi.org/10.5194/egusphere-egu26-6673, 2026.

EGU26-6716 | Orals | EMRP2.8

Large, Long-lasting Mid-Latitude Geomagnetically Induced Currents During a Moderate Geomagnetic Storm 

Andy Smith, Craig Rodger, Jonathan Rae, John Coxon, Daniel Mac Manus, Johnny Malone-Leigh, Mark Clilverd, Colin Forsyth, Ciaran Beggan, Kristin Pratscher, Gemma Richardson, Andrew Dimmock, Juliane Huebert, Tanja Petersen, Andrew Renton, Michael Dalzell, and Maria-Theresia Walach

Large Geomagnetically Induced Currents (GICs) are a key space weather hazard to ground-based infrastructure.  These GICs act as a DC offset in typically AC power networks and when very large can cause mis-operation or even equipment failure.  The dynamic solar wind interacts with the Earth’s geomagnetic field, causing the magnetic field as measured on the ground to vary with time.  Via coupling with the geology of the solid Earth, this variability causes GICs to be created in grounded conducting networks.  Most studies of the GIC hazard focus on short, fast changes of the geomagnetic field, for example large “spikes” in the one-minute rate of change of the horizontal geomagnetic field.

However, recent work has reminded researchers that long intervals of lower (relative) GIC can also be problematic, and represents a known pathway to equipment damage and long-lasting power failure.  In this study we evaluate a curious interval where the power network in New Zealand experienced long duration, steadily increasing GICs across the South Island.  These GICs were up to 20 A and lasted approximately 90 minutes, manifesting in the mid-latitude dawn sector during an otherwise moderate geomagnetic storm.  We investigate the magnetospheric cause of the ground observations, and the ability of contemporary modelling techniques to capture this facet of the GIC hazard to ground-based infrastructure.  Further, this case study highlights the limitations of geomagnetic indices, which we show to be vulnerable to contamination from such rare mid-latitude phenomena.

How to cite: Smith, A., Rodger, C., Rae, J., Coxon, J., Mac Manus, D., Malone-Leigh, J., Clilverd, M., Forsyth, C., Beggan, C., Pratscher, K., Richardson, G., Dimmock, A., Huebert, J., Petersen, T., Renton, A., Dalzell, M., and Walach, M.-T.: Large, Long-lasting Mid-Latitude Geomagnetically Induced Currents During a Moderate Geomagnetic Storm, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6716, https://doi.org/10.5194/egusphere-egu26-6716, 2026.

Long-period obliquity modulation can drive low-frequency hydroclimate variability by changing meridional insolation gradients and influencing the position and intensity of the East Asian monsoon rainband. What is less clear is how consistently such low-frequency signals are captured across different fine-grained depositional settings. Here we compare two end-member archives along the East Asian continental foreland: (i) dust-derived aeolian red clays in semi-arid regions near desert source areas, and (ii) organic-rich black shales deposited in more moisture-proximal settings, from lakes to shallow seas. The depositional processes are different, but both archives often damp higher-frequency noise and preserve long-period orbital pacing, which makes them useful for evaluating the timing and spatial pattern of monsoon-related hydroclimate change.

In the northern late Eocene red-clay succession from the eastern Mongolian Plateau, rock-magnetic and geochemical proxies show pronounced orbital-scale variability between ~48 and 36 Ma. Obliquity-paced modulation is clear, and wetter intervals cluster around high-obliquity nodes. The site sits in a continental-foreland position where moisture delivery from the south and southeast is likely sensitive to north–south shifts of the monsoon rainband and associated subtropical circulation changes.

For a deeper-time shale endmember, we examine Middle Triassic black-shale successions formed during warming and broader Earth-system reorganization. At that time, the North China and South China blocks lay along the eastern margin of Pangea, facing the ocean and remaining sensitive to changes in moisture supply. Geochemical series and magnetic susceptibility from lacustrine to shallow-marine settings show strong obliquity modulation, expressed as a ~1.2 Myr envelope with embedded ~173 kyr variability, together with a 405 kyr band. These patterns suggest that the ~1.2 Myr and ~173 kyr obliquity components can organize rainfall variability in both continental and marine fine-grained archives, and that this behavior extends back to at least ~250 Ma.

Next, using published evidence for cyclicity in Eocene shales from the East China Sea region, we will test whether similar long-period obliquity bands occur in Eocene marine black shales and whether their phases match those in the terrestrial red-clay record. Comparing red clays and black shales as products of a land–sea moisture gradient, using environmental magnetism together with cyclostratigraphy, offers a direct way to connect shale formation and monsoon climate forcing.

How to cite: Zhang, S. M.: Obliquity-modulated East Asian monsoon variability recorded coherently in fine-grained red clays and black shales across a land–sea moisture gradient, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8289, https://doi.org/10.5194/egusphere-egu26-8289, 2026.

EGU26-8660 | ECS | Posters on site | EMRP2.8

New Cambrian paleomagnetic constraints on South China Block paleogeography and Gondwana linkages  

Dongmeng Zhang, Xin Cheng, Vadim A. Kravchinsky, and Hanning Wu

The Early Paleozoic paleogeographic position of the South China Block (SCB) and its affinity with Gondwana remain contentious. This study presents new, high-quality paleomagnetic data from Cambrian Stage 3 clastic rocks (Kunming, southwestern SCB) that quantitatively constrain its early Paleozoic paleogeography.

Systematic analyses identify a primary remanent magnetization carried by detrital magnetite. This component passes fold and reversal tests, shows no significant inclination shallowing, and averages out secular variation. Following a regional Cenozoic rotation correction, the paleopole positions the SCB at a paleolatitude of ~13.6°S at ~518 Ma. This location places its outhwestern margin adjacent to the western margin of East Gondwana. Paleogeographic reconstructions illustrate a contiguous spatial relationship and a concordant margin orientation between the two blocks. 

Our new paleomagnetic pole, supported by existing paleobiogeographic and provenance data, firmly establishes the SCB as a constituent part of East Gondwana from the Early Cambrian to Early Devonian (~520–405 Ma). These results provide robust evidence for refining Cambrian paleogeographic models of Gondwanan assembly.

How to cite: Zhang, D., Cheng, X., Kravchinsky, V. A., and Wu, H.: New Cambrian paleomagnetic constraints on South China Block paleogeography and Gondwana linkages , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8660, https://doi.org/10.5194/egusphere-egu26-8660, 2026.

EGU26-8676 | Posters on site | EMRP2.8

A High-Precision GPS/BeiDou-Synchronized Proton Precession Magneto 

Nur Ailie Sofyaiana Binti Serasa, Wenwen Chang, Yugang Zhao, and Huang Shenshuo

With the advancement of science and technology and the development of human society, there is an increasing demand for higher precision in magnetic field measurement. The proton precession magnetometer is precisely such an instrument capable of accurately measuring the geomagnetic field. As a high-precision magnetic field measuring device, it has been widely applied in high-precision magnetic surveys, mineral exploration, tectonic detection, seismic and volcanic precursor observation, engineering and environmental exploration, coalfield and hydrogeological exploration, pipeline and underground explosive detection, archaeology, petroleum and natural gas exploration, and other industries, thanks to its stable performance, compact size, ease of portability and simple operation.

This paper introduces a high-precision proton precession magnetometer developed by Beijing Orangelamp Geophysical Exploration Co., Ltd., with a detailed description and analysis of its working principle, appearance, functions, operation procedures and performance tests. This high-precision proton precession magnetometer has been widely used in the Chinese market and has received favorable feedback.

The high-precision proton precession magnetometer described in this paper adopts GPS or BDS (BeiDou Navigation Satellite System) for time synchronization, eliminating the tedious process of manual time input. In a favorable magnetic field environment, its noise level can reach 0.05 nT. Moreover, it is compatible with a dedicated free magnetic data processing software package developed by Beijing Orangelamp Geophysical Exploration Co., Ltd. The absolute error of this proton precession magnetometer is also controlled within ±0.5 nT.

How to cite: Binti Serasa, N. A. S., Chang, W., Zhao, Y., and Shenshuo, H.: A High-Precision GPS/BeiDou-Synchronized Proton Precession Magneto, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8676, https://doi.org/10.5194/egusphere-egu26-8676, 2026.

EGU26-9029 | Posters on site | EMRP2.8

Application of Cesium Optical Pump UAV Aeromagnetic System in Coastal Shallow Water Areas 

Yinze Wang and Wenwen Chang

Aerogeophysical survey is an exploration method that uses aircraft as the carrier, carries geophysical prospecting instruments to detect geophysical field information during flight, and studies the internal structure and material composition of the Earth based on the collected data to solve geological problems. This method is not restricted by terrain and enables efficient and rapid survey operations. At present, the application of low-altitude magnetic survey in iron ore exploration has become quite mature in China. Unmanned aerial vehicle (UAV) aeromagnetic systems are also increasingly sophisticated in such fields as onshore mineral resource exploration and geological structure survey, but their application in marine surveys is still in the initial stage.

The working principle of aeromagnetic survey is that the UAV carries magnetic sensors for magnetic field observation, which specifically consists of seven components: 1. Flight carrier system; 2. Airborne aeromagnetic survey system; 3. Ground control station; 4. Ground magnetic diurnal variation base station; 5. Work auxiliary equipment; 6. Field data preprocessing system; 7. Data interpretation system.

This paper mainly introduces the application of aeromagnetic survey in nearshore submarine pipeline detection. The UFO-CS multi-rotor cesium optical pump aeromagnetic survey system, independently developed and manufactured by Beijing Orangelamp Geophysical Exploration Co., Ltd., is adopted for measurement and data interpretation in this application.

How to cite: Wang, Y. and Chang, W.: Application of Cesium Optical Pump UAV Aeromagnetic System in Coastal Shallow Water Areas, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9029, https://doi.org/10.5194/egusphere-egu26-9029, 2026.

EGU26-9176 | ECS | Posters on site | EMRP2.8

Investigation of Geomagnetically Induced Current activity indices using Information Theory 

Adamantia Zoe Boutsi, Pouya Manshour, Constantinos Papadimitriou, Georgios Balasis, and Milan Palus

Geomagnetically Induced Currents (GICs) are a manifestation of space weather events at ground level. GICs have the potential to cause power failures in electric grids. The GIC index is a proxy of the ground geoelectric field derived solely from geomagnetic field data. Information Theory (IT) can be used to shed light on the dynamics of complex systems, such as the coupled solar wind-magnetosphere-ionosphere-ground system. Previously, we have performed block entropy analysis of the GIC activity indices at middle-latitude European observatories around the St. Patrick's Day March 2015 intense magnetic storm and Mother's Day (or Gannon) May 2024 super-intense storm. We found that the GIC index values were generally higher for the May 2024 storm, indicating elevated risk levels. Furthermore, the entropy values of the SYM-H and GIC indices were higher in the time interval before the  storms than during the storms, indicating transition from a system with lower organization to one with higher organization. Recently, IT has proven itself as a powerful approach to study causal relationships among various coupled complex systems. Here, we use Conditional Mutual Information as a measure of causality which is, indeed, the mutual information between the cause and the future of the effect variable, conditioned on the history of the effect variable, to investigate the possible coupling direction and pattern of interactions among different GIC indices, and various solar wind variables and geomagnetic activity indices.

How to cite: Boutsi, A. Z., Manshour, P., Papadimitriou, C., Balasis, G., and Palus, M.: Investigation of Geomagnetically Induced Current activity indices using Information Theory, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9176, https://doi.org/10.5194/egusphere-egu26-9176, 2026.

EGU26-9315 | ECS | Posters on site | EMRP2.8

A Study on the Dynamic Nuclear Polarization Efficiency of a Novel Nitroxide Radical 

Yujie Jiang and Xiangjun Li

Abstract: Nuclear magnetic resonance (NMR) mapping, valued for its non‑destructive nature and high resolution, is extensively employed in geological exploration to analyze the distribution of geological structures, mineral resources, and other subsurface targets. However, the intrinsic low sensitivity of NMR limits its utility in weak‑signal environments. Dynamic nuclear polarization (DNP) overcomes this constraint by using radiofrequency excitation to transfer polarization from electron spins to nuclear spins. This mechanism effectively relays the high polarization of electrons to the nuclear spin system, markedly boosting NMR detection sensitivity and serving as a pivotal signal‑enhancement strategy.

Within DNP systems, nitroxide radicals are widely studied due to their chemical stability and synthetic accessibility. However, their polarization efficiency is often limited by the magnetic transition characteristics of the conventional nitrogen nucleus. To address this, the present study established an electron paramagnetic resonance (EPR) spectral simulation method based on software such as Gaussian and ORCA. Guided by this approach, a novel nitroxide radical was designed and synthesized with the aim of enhancing DNP performance at low to medium magnetic fields. EPR experimental results show that this radical exhibits a narrow EPR linewidth and higher unpaired electron transition intensity compared to conventional nitroxide radicals. These properties enable it to overcome the electron transition energy limitations of conventional nitroxide radicals under medium- and low-field conditions, thereby achieving a higher nuclear polarization rate.

In conclusion, this study introduces an efficient design strategy centered on a novel nitroxide radical, which substantially improves DNP signal enhancement and supports the advancement of NMR mapping technology.

How to cite: Jiang, Y. and Li, X.: A Study on the Dynamic Nuclear Polarization Efficiency of a Novel Nitroxide Radical, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9315, https://doi.org/10.5194/egusphere-egu26-9315, 2026.

EGU26-9977 | Posters on site | EMRP2.8

Evidence of Interhemispheric Asymmetry in Swarm Geomagnetic Activity Indices Using Complexity Measures 

Constantinos Papadimitriou, Georgios Balasis, Adamantia Zoe Boutsi, and Ioannis A. Daglis

Swarm data can be used to derive spaceborne indices of geomagnetic activity, capturing the same dynamic processes and exhibiting the same behaviour as ground-based geomagnetic indices traditionally used to monitor magnetic storm (SYM-H index) and substorm (AE index) activity. Given the fact that the official ground-based index for the substorm activity (i.e., the Auroral Electrojet – AE index) is constructed by data from 12 ground stations, solely in the northern hemisphere, it can be said that this index is predominantly northern, while the Swarm-derived AE index may be more representative of a global state, since it is based on measurements from both hemispheres. A few studies have addressed the question of whether the auroras are symmetric, between the northern and southern hemispheres. Therefore, the possibility to have different Swarm-derived AE indices for the northern and southern hemispheres respectively, may provide, under appropriate time series analysis techniques based on information theoretic approaches, an opportunity to further confirm the recent findings on interhemispheric asymmetry. Here, we also provide evidence for interhemispheric energy asymmetry in the ionosphere based on the analyses of Swarm-derived auroral indices AE North and AE South.

How to cite: Papadimitriou, C., Balasis, G., Boutsi, A. Z., and Daglis, I. A.: Evidence of Interhemispheric Asymmetry in Swarm Geomagnetic Activity Indices Using Complexity Measures, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9977, https://doi.org/10.5194/egusphere-egu26-9977, 2026.

EGU26-10283 | Posters on site | EMRP2.8

From Seed Fields to Magnetism in Planets and Galaxies 

Angelo De Santis, Roberto Dini, and Gianfranco Cianchini

This study explores the origin and evolution of magnetic fields in planetary bodies and galaxies, focusing on the role of an initial seed magnetic field (SMF) required for dynamo operation. We propose a general physical mechanism in which a seed field arises naturally in systems where an orbiting body rotates non-synchronously relative to its central mass. Building on this idea, we derive a unified formulation for the SMF that is applicable across both planetary and galactic scales and incorporates fundamental parameters such as orbital distance, rotational velocity, and core radius. To relate the seed field to observed magnetic field strengths, we introduce a dimensionless parameter that represents the efficiency of dynamo amplification. Model predictions are compared with magnetic field measurements from the solar system and the Milky Way. The results suggest that observed magnetic fields can be interpreted as the product of a universal, gravity-induced seed field and a system-dependent amplification factor. This framework offers a complementary perspective on magnetic field generation in a wide range of astrophysical environments and highlights potential implications for magnetism in extreme settings, including regions surrounding black holes.

How to cite: De Santis, A., Dini, R., and Cianchini, G.: From Seed Fields to Magnetism in Planets and Galaxies, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10283, https://doi.org/10.5194/egusphere-egu26-10283, 2026.

EGU26-13735 | Posters on site | EMRP2.8

From loess to deep-time red clays: magneto-cyclostratigraphy reveals orbital pacing in East Asian dust archives back to ~60 Ma 

Rui Zhang, Minghao Ma, Hujun Gong, leonardo Sagnotti, and Vadim A. Kravchinsky

Eolian red clays provide one of the few terrestrial archives that can track East Asian dust transport and hydroclimate variability beyond the Quaternary loess–paleosol sequence. Over the past decades, a growing body of magnetostratigraphic and cyclostratigraphic work has steadily pushed the upper age limit of astrochronologically resolved eolian red-clay records from the familiar ~3 Ma interval on the Chinese Loess Plateau to much older Cenozoic time slices. Here we synthesize this stepwise extension and highlight how environmental magnetism has been central to establishing an orbital-scale stratigraphic framework across a wide range of source–sink settings.

On the Loess Plateau, orbital-scale variability is well expressed in magnetic susceptibility and related rock-magnetic parameters, enabling robust dating over the late Neogene (~8 Ma) and, in the western Plateau, into the early Miocene (>20 Ma). Subsequent discoveries farther west expanded the record dramatically: red-clay successions near the eastern margin of the Tibetan Plateau (Altun region) preserve orbitally paced variability back to ~50 Ma, while sections along the northern Junggar Basin extend to ~25 Ma. In the eastern Erlian Basin (Inner Mongolia), continuous fine-grained red clays document cyclicity reaching at least ~48 Ma. Most recently, even older Cenozoic eolian red-clay sequences (~60 Ma) have been identified by us in the Qinling region, suggesting that dust-bearing winds and low-frequency hydroclimate pacing were established early in the Cenozoic and remained persistent across shifting paleogeography and boundary conditions.

Across these regions, magnetic susceptibility and complementary rock-magnetic proxies consistently capture astronomical forcing, with prominent long-period eccentricity and obliquity modulation embedded within precession-scale variability, despite clear differences in depositional setting, distance to desert sources, and post-depositional alteration. Treating the Cenozoic red-clay belt as a spatially distributed “network” of archives allows us to (i) test the reproducibility and phase stability of orbital signals across basins, (ii) evaluate how dust supply and pedogenic processes filter orbital forcing, and (iii) refine Cenozoic terrestrial timescales where independent radiometric constraints are limited. This synthesis shows that Cenozoic eolian red clays, when anchored by magnetostratigraphy and analyzed with cyclostratigraphy, can provide a coherent astrochronological framework from ~3 to ~60 Ma and open a path to reconstruct long-term East Asian dust–monsoon evolution on orbital timescales.

How to cite: Zhang, R., Ma, M., Gong, H., Sagnotti, L., and Kravchinsky, V. A.: From loess to deep-time red clays: magneto-cyclostratigraphy reveals orbital pacing in East Asian dust archives back to ~60 Ma, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13735, https://doi.org/10.5194/egusphere-egu26-13735, 2026.

EGU26-14023 | Posters on site | EMRP2.8

The MARGE magnetotelluric array in Central Italy: measurements and modelling perspectives for geomagnetic applications and geoelectric hazard assessment  

Paola De Michelis, Marianna Balasco, Igino Coco, Michele De Girolamo, Manuele Di Persio, Fabio Giannattasio, Cesidio Gizzi, Valerio Materni, Luca Miconi, Massimo Miconi, Giovanna Lucia Piangiamore, Giulia Pigniatiello, Gerardo Romano, Valentina Romano, Lucia Santarelli, Vincenzo Sapia, Sabina Spadoni, Roberta Tozzi, Simona Tripaldi, and Agata Siniscalchi

Rapid variations of the geomagnetic field represent both a resource and a hazard for modern technological systems. While geomagnetic observations support a wide range of applications, from navigation to positioning, storm-time magnetic disturbances can induce strong geoelectric fields at the Earth’s surface, driving geomagnetically induced currents (GICs) that threaten power grids and other grounded infrastructures. Accurate modelling of these ground effects critically depends on realistic representations of the Earth’s electrical conductivity.

In this contribution, we present the first results from the MARGE (Magnetotelluric ARray in Central Italy for GEoelectric hazard assessment) project, a measurement-driven initiative designed to provide the geophysical foundation for geomagnetic applications related to space-weather impacts. MARGE consists of a broadband and long-period magnetotelluric (MT) array deployed on a ~50 km grid across central Italy, a region characterized by strong lateral conductivity contrasts associated with active tectonics, sedimentary basins, volcanic provinces, and land–sea boundaries.

We describe the survey design, instrumentation, and data processing strategy, and assess the quality of 20 MT soundings acquired between 2023 and 2025. More than 75% of the sites yield good to excellent impedance estimates over periods from 10-3 to 104 s. Apparent resistivity, phase curves, and phase tensor analysis reveal pronounced spatial and depth-dependent variability of the electrical structure, highlighting the inadequacy of simplified one-dimensional conductivity models for geomagnetic applications in this region.

These first measurement-based results demonstrate the feasibility of constructing a realistic 3-D conductivity framework for Italy and represent a key step toward physics-based modelling of storm-time geoelectric fields. MARGE provides essential input for future GIC simulations and contributes to improving the reliability of geomagnetic-field-based applications and risk mitigation strategies.

How to cite: De Michelis, P., Balasco, M., Coco, I., De Girolamo, M., Di Persio, M., Giannattasio, F., Gizzi, C., Materni, V., Miconi, L., Miconi, M., Piangiamore, G. L., Pigniatiello, G., Romano, G., Romano, V., Santarelli, L., Sapia, V., Spadoni, S., Tozzi, R., Tripaldi, S., and Siniscalchi, A.: The MARGE magnetotelluric array in Central Italy: measurements and modelling perspectives for geomagnetic applications and geoelectric hazard assessment , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14023, https://doi.org/10.5194/egusphere-egu26-14023, 2026.

Alternative magnetic navigation (aka MagNav) depends on matching of onboard sensor readings with prior mapping of the Earth’s magnetic field. Three critical components to successful MagNav are (1) sensor accuracy, (2) magnetically clean sensor platform with compensation for any residual platform effects, and (3) reference map quality. Relatively inexpensive magnetic sensors are sufficient for successful MagNav. Established methods are sufficient to calibrate all but the noisiest platforms. The purpose of this presentation is to dig into (3); specifically, how to assess the quality of directional magnetic anomaly gradients (DMAG) from magnetic maps and deliver the most reliable reference values to nav systems. At each navigation time step a comparison is made between the measured and mapped gradients. Successful MagNav depends on the ability to quantify the level of match between these values. A critical component is an understanding of the characteristics of uncertainty in the estimation of DMAG for input to the navigation filter algorithm.

Current navigation systems ingest magnetic map data as a “stack of grids” prepared from an original survey grid by upward continuation (typically using an FFT method). Anomaly values and east-west/north-south gradients are interpolated from these grids for comparison with magnetic sensor data in the navigation filter. The reliability of these anomaly and gradient values is dependent on several factors, including the uncertainty in the original survey grid, edge effects or other artefacts from upward continuation, and method of grid interpolation. The use of an equivalent source model instead of a stack of static grids offers opportunities for uncertainty propagation and ability to query anomaly and gradient values and related uncertainty at arbitrary locations and cadence. The purpose of this presentation is to give comparative examples of DMAG evaluations using different methods applied to synthetic and actual data.

How to cite: Saltus, R., Chulliat, A., and Califf, S.: Navigating from Magnetic Maps – Improving Reliability of Magnetic Anomaly and Gradient Reference Values from Imperfect Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14369, https://doi.org/10.5194/egusphere-egu26-14369, 2026.

EGU26-15080 | Orals | EMRP2.8

Induced Geoelectric Fields as a Key Space Weather Variable 

Martin Connors, Ian Schofield, and Darcy Cordell

Many of the effects of geomagnetic field variations, apart from those on devices using the geomagnetic field directly, are through induction of electric fields as described by Faraday’s Law. Such electric fields in turn cause an Ohmic effect in the Earth and conducting infrastructure, giving rise to potentially harmful geomagnetically induced currents (GIC). Precise measurement of the geomagnetic field dates back nearly two centuries, but localized measurements of geoelectric fields started mostly with magnetotelluric prospecting only in the mid-twentieth century. For this historical reason, and due to measuring difficulties now circumvented by modern technology, direct detection of geoelectric fields for space weather applications has rarely been done. We will describe efforts at Athabasca University to measure geomagnetic and geoelectric fields with a wide range of equipment, from commercial coil-based systems at 2400 Hz to extremely inexpensive systems based on microcontrollers and analog front ends. In principle, geoelectric field measurement devices can be simplified, and made inexpensive, more readily than those for geomagnetic fields, making networks of them a good way to monitor localized GIC effects. Recent cases of detection of large geoelectric fields in our region will be discussed.

How to cite: Connors, M., Schofield, I., and Cordell, D.: Induced Geoelectric Fields as a Key Space Weather Variable, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15080, https://doi.org/10.5194/egusphere-egu26-15080, 2026.

Extremely high-energy SEPs, which attain energies in the GeV range, are accelerated during impulsive solar flares and in association with CMEs. These relativistic particles represent a primary driver of hazardous space weather phenomena. They pose significant risks to spacecraft operations and crew safety during deep-space missions, while also threatening ground-based infrastructure, particularly power grids and other critical components of the electromagnetic environment, through geomagnetic disturbances and induced currents. Spectral observations indicate that the acceleration of SEPs to GeV energies involves highly complex, multi-component processes characterized by diverse ion compositions. The particle population predominantly comprises hydrogen (protons and electrons, approximately 73%), helium (approximately 25%), and heavier ions. Notably, the mass-to-charge ratio (A/Q) differs markedly between helium isotopes: 1.5 for ³He²⁺ and 2.0 for ⁴He²⁺.

 

In the present study, we examine the acceleration processes and ³He enrichment in SEP events within a statistical plasma-physics framework integrated with turbulence theory. Our methodology explicitly accounts for the realistic proton-to-electron mass ratio, the distinct mass-to-charge ratios of relevant ion species, and the effects of turbulence resistivity and viscosity. These elements are incorporated into a fully coupled hydrodynamics–magnetohydrodynamics–kinetic model that bridges continuous spatial and temporal scales, thereby circumventing the traditional separation of micro-kinetic and macro-dynamic regimes.

 

Numerical simulations are conducted on a supercomputer using our newly developed relativistic hybrid particle-in-cell and lattice-Boltzmann method (RHPIC-LBM) code. This advanced computational approach facilitates self-consistent modeling of the multi-scale, multiphase dynamics underlying the extreme ³He enhancements observed in impulsive solar SEP events. The simulations reveal that high-frequency magnetic fluctuations at kinetic scales play a pivotal role in generating self-organized perturbations. Concurrently, plasma velocity fluctuations sustain and amplify these waves through self-feeding mechanisms. When the frequency of these perturbations approaches the Langmuir oscillation frequency, resonant wave–particle interactions become particularly efficient. Langmuir turbulence, driven by nonlinear resonant wave–particle coupling, preferentially accelerates ions whose resonance conditions match those of ³He. This selective resonance renders the acceleration of ³He substantially more efficient than that of ⁴He, thereby providing a compelling explanation for the extreme ³He enrichment characteristic of impulsive SEP events.

How to cite: Li, Y., Zhu, B., and Zhao, Y.: ³He Enrichment in SEP Events: Observational Constraints and Evidence from Isotopic Fractionation via Resonant Wave–Particle Interactions and Turbulent Acceleration, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16097, https://doi.org/10.5194/egusphere-egu26-16097, 2026.

Solar Cycle 25 has exceeded initial intensity predictions, characterized by a series of severe geomagnetic disturbances that have expanded the auroral oval well into mid-latitudes. This study presents a comparative analysis of the magnetospheric and ionospheric responses to three distinct events observed over the European sector, including regions such as Türkiye: the geomagnetic storms of November 2023, May 2024, and October 2024. By integrating Global Navigation Satellite System (GNSS)–derived Total Electron Content (TEC) data with ground-based magnetometer observations, the spatiotemporal evolution of these disturbances is characterized. All three events were driven by Coronal Mass Ejections (CMEs), yet their impacts on the mid-latitude ionosphere differed substantially. The May 2024 extreme storm was marked by prolonged negative ionospheric phases and severe TEC depletions over Europe, including Türkiye, primarily linked to compositional changes and disturbance dynamo electric fields (DDEFs). In contrast, the November 2023 storm exhibited coherent magnetic field depressions and rapid recovery phases, indicating a dominant role of prompt penetration electric fields (PPEFs). This comparative framework is extended to the October 2024 storm. Moreover, analysis of the vertical (Z) and horizontal (H) geomagnetic field components recorded at European observatories provides insight into the penetration of high-latitude current systems into lower latitudes during intense space weather events. The results demonstrate that mid-latitude regions experience complex electrodynamic coupling during the solar cycle maximum, governed by multiple mechanisms ranging from prompt electric field penetration to thermospheric heating across the Eastern Mediterranean sector.

How to cite: Çiftçi, E., Hacıoğlu, Ö., and Kotan, B.: Auroral Signatures of Solar Cycle 25 at Mid-Latitudes: A Comparative Analysis of the November 2023, May 2024, and October 2024 Geomagnetic Storms, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16268, https://doi.org/10.5194/egusphere-egu26-16268, 2026.

EGU26-16734 | ECS | Posters on site | EMRP2.8

Linking Broadband Magnetotelluric Impedance, Magnetic Variations, and Geoelectric Field Dynamics in Severe Storms 

Michele De Girolamo, Paola De Michelis, Giulia Pigniatiello, Elettra Consolini, and Agata Siniscalchi

Geomagnetically induced currents pose a well-recognized risk to ground-based technological systems during periods of intense geomagnetic activity. A key step in quantifying this risk is the reconstruction of the storm-time geoelectric field, which is controlled by the electrical conductivity structure of the subsurface. Although long-period magnetotelluric (MT) surveys provide optimal constraints for this purpose, many regions are covered primarily by legacy broadband MT datasets acquired for geological investigations and rarely exploited in a space-weather context. In this study, we investigate whether archived broadband MT data can be effectively used to estimate geoelectric fields relevant for GIC studies. We focus on the two most severe geomagnetic storms of 2024 (May and October), combining a broadband MT impedance tensor derived from three years of observations at the Gargano station (southern Italy) with 1 Hz magnetic field measurements from the nearby Duronia geomagnetic observatory. The analysis targets the 2–8000 s period range, which dominates GIC generation. Modeled electric field components are independently evaluated by comparison with storm-time electric field measurements decomposed into intrinsic mode functions using Empirical Mode Decomposition. The consistency between modeled and observed signals is assessed through Mutual Information analysis, revealing a statistically significant correspondence, particularly during storm main phases. These results show that legacy broadband MT datasets can provide quantitative and physically meaningful estimates of storm-time geoelectric fields. Existing MT archives therefore offer a valuable and cost-effective opportunity for preliminary GIC hazard assessment and retrospective space weather analyses, especially in regions lacking dedicated long-period MT coverage. This research was funded by the Space It Up! project funded by the Italian Space Agency, ASI, and the Ministry of University and Research, MUR, under contract n. 2024-5-E.0—CUP n.I53D24000060005.

How to cite: De Girolamo, M., De Michelis, P., Pigniatiello, G., Consolini, E., and Siniscalchi, A.: Linking Broadband Magnetotelluric Impedance, Magnetic Variations, and Geoelectric Field Dynamics in Severe Storms, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16734, https://doi.org/10.5194/egusphere-egu26-16734, 2026.

EGU26-17750 | Orals | EMRP2.8

Space Weather Impacts on Railway Systems 

Cameron Patterson and Jim Wild

Railways rely on interdependent systems for power, navigation, communications, and signalling, many of which are at risk of being impacted by space weather. Understanding how and to what extent space weather can impact these systems is crucial to maintaining the safe and reliable operation of railway networks.

Power supply disruption would leave trains on electrified lines stranded and can disrupt signalling operations, while geomagnetically induced currents introduced into the AC-electrified overhead line equipment can affect locomotive on-board transformers. GNSS disturbances can interfere with high-speed trains’ tilt control systems, limiting their speed and leading to delays. Loss of service of GSM-R (Global System for Mobile Communications Railway), which is used for communications and is an integral part of the advanced ETCS (European Train Control System), would impact operations. DC track circuit signalling systems on AC-electrified lines are susceptible to interference from geomagnetically induced currents which can lead to incorrect signals, causing delays or, in the worst case, collisions.

This presentation aims to provide an overview on our understanding of space weather impacts on railway systems, highlight recent work and identify potential avenues for future study.

How to cite: Patterson, C. and Wild, J.: Space Weather Impacts on Railway Systems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17750, https://doi.org/10.5194/egusphere-egu26-17750, 2026.

EGU26-19540 | ECS | Orals | EMRP2.8

Refined Modeling of Ionospheric Induction During the 24 October 2011 Sudden Commencement 

Andreas Sæther Skeidsvoll, Karl Magnus Laundal, Spencer Mark Hatch, Michael Madelaire, Beatrice Popescu Braileanu, and Fasil Tesema Kebede
Conventional approaches to magnetosphere-ionosphere-thermosphere (MIT) coupling frequently employ a steady-state approximation. However, this assumption is likely insufficient for characterizing the system's response to highly dynamic events. In this study, we utilize a global, two-dimensional model that incorporates ionospheric induction. Recent refinements to the model have yielded higher spatial resolution and improved stability in the interhemispheric coupling regions.
 
We apply this model to the 24 October 2011 sudden commencement, driving the simulation with time-dependent output from the MAGE model. We isolate the specific contribution of induction by comparing the results to a non-inductive baseline, and we validate the dynamic response against ground magnetometer measurements. The analysis reveals that induction produces an ionospheric response that is significantly delayed and dampened relative to the steady-state solution. We discuss how the model allows for a more rigorous interpretation of ground magnetic perturbations and outline the requirements for extending this scheme to fully coupled, two-way simulations.

How to cite: Skeidsvoll, A. S., Laundal, K. M., Hatch, S. M., Madelaire, M., Popescu Braileanu, B., and Tesema Kebede, F.: Refined Modeling of Ionospheric Induction During the 24 October 2011 Sudden Commencement, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19540, https://doi.org/10.5194/egusphere-egu26-19540, 2026.

EGU26-21137 | Orals | EMRP2.8

Magnetic field coupling across the Earth system as screened by the ionosphere 

Octav Marghitu, Mioara Mandea, Elvira Astafyeva, and George Balasis

From its core to the magnetosphere and further into the solar wind, the Earth system is tightly coupled and the magnetic field is the glue that mediates the coupling. At the same time, the ionosphere behaves as a huge natural screen, where phenomena from above and below provide a broad range of complicated signatures, mapped along the magnetic field. The proper reading and disentangling of these signatures have a major potential to advance the fundamental understanding of the coupled Earth ‘spheres’ as well as of a vast set of applications and tools, covering from space weather and natural hazards to effects on space-borne and ground-based technology. While this is in principle well understood, the actual handling of the ionospheric observations and the tracing of the true sources behind ionospheric disturbances is often most challenging. The presentation will illustrate a few examples, emphasizing the major importance of the magnetic field in providing the coupling, of the ionosphere in screening it, and of a systematic approach yet to be done.

How to cite: Marghitu, O., Mandea, M., Astafyeva, E., and Balasis, G.: Magnetic field coupling across the Earth system as screened by the ionosphere, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21137, https://doi.org/10.5194/egusphere-egu26-21137, 2026.

The success of marine magnetics to date the seafloor and reconstruct the evolution of basins in not to demonstrate anymore.  However, some basins still remain poorly understood, either because of limited data coverage, tectonic complexity, or narrow width that do not allow full sequences of recognizable magnetic anomalies to be clearly identified.  We propose new approaches that add to the classical identification of geomagnetic polarity reversal including the interpretation of tiny wiggles, i.e., low amplitude short wavelength anomalies that reflect paleointensity variations, and long wavelength anomalies that, in the absence of magnetized extrusive basalt, represent the contribution of the deeper oceanic crust. Examples of sea-surface and near-seafloor data where these approaches have helped to solve dating and reconstructing oceanic basin history will be presented.

How to cite: Dyment, J.: Marine magnetics: new approaches to solve plate tectonic problems in complex or narrow basins, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21480, https://doi.org/10.5194/egusphere-egu26-21480, 2026.

EMRP3 – Paleomagnetism and Environmental Magnetism

EGU26-449 | ECS | Posters on site | EMRP3.2

Flow direction and internal structure of Seaward Dipping Reflectors along the Mid-Norwegian Volcanic Margin 

Pradyut Phukon, Amar Agarwal, Natalia Varela, Mamilla Venkateshwarlu, and Eric C. Ferré

The Mid-Norwegian margin hosts a thick volcanic succession of break-up–related basalts forming the seaward-dipping reflectors (SDRs). We investigated the magnetic fabric of basalts sampled from the feather edge of inner SDR packages. Azimuthally unoriented samples were collected during International Ocean Drilling Program (IODP) Expedition 396, from three sites along the margin from Kolga High in the south to the Skoll High in the north. Rock magnetic characterization suggests the presence of pseudo-singe domain Ti-magnetite as the main remanence carrier in the basalt. Our results show that the AMS in SDR basalt primarily reflects distribution anisotropy arising from subhedral/euhedral Ti-magnetite grains enclosed within an early-formed silicate framework.

The direction of natural remanent magnetization (NRM) preserved in the basalts is used to reorient the specimens into their in-situ orientation, allowing interpretation of the AMS fabric in a geographic coordinate system. Reoriented magnetic fabrics show systematic alignment with independent flow indicators.

Individual lava flows exhibit a strong zonation of magnetic fabric, characterized by oppositely dipping foliations in the top and basal parts. The opposing pair of foliations is attributed to flow-induced shear strain that is effective in the distal parts, away from the eruption centre, once a semi-solid / solid upper crust is developed. Imbricated magnetic foliations developed at the base of individual flows are used to decipher the lava flow direction, which indicates a consistently landward-directed lava transport towards the south. AMS-derived flow directions are also supported by seismic images, which show subvertical dyke swarms at the seaward edge of the inner SDR in the north, that likely served as feeders to the thick basaltic succession.

How to cite: Phukon, P., Agarwal, A., Varela, N., Venkateshwarlu, M., and Ferré, E. C.: Flow direction and internal structure of Seaward Dipping Reflectors along the Mid-Norwegian Volcanic Margin, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-449, https://doi.org/10.5194/egusphere-egu26-449, 2026.

EGU26-587 | ECS | Posters on site | EMRP3.2

Shock Effects on Magnetic Remanence in Rocks from the Dhala Impact Structure, India 

Ambrish Kumar Pandey, Amar Agarwal, Satish J. Sangode, and Gaurav Joshi

Impact-generated shock waves can modify the remanence properties of magnetic minerals in target rocks, but their effects remain poorly understood. This study examines shock-induced modifications in the magnetic properties of both unshocked lithologies and impactites at the Dhala impact structure in India. The structure formed during the Paleoproterozoic (2.5–1.7 Ga) and lies within the Bundelkhand craton of the Indian Shield, with an original diameter of ~11 km. The unshocked target lithologies are primarily granitoid, while two types of impactites, impact melt rock and monomict breccia, are prominently exposed at the surface. Primary magnetic carriers are multidomain (MD) Ti-poor magnetite in unshocked rocks; pseudo–single-domain (PSD) Ti-magnetite with minor Ti-hematite and pyrrhotite in impact melt rock; and pseudo–single-domain to single-domain (PSD–SD) Ti-magnetite with minor Ti-hematite in monomict breccia (Pandey et al., 2026). To evaluate coercivity spectra, domain state, and remanence efficiency, alternating field (AF) demagnetization, isothermal remanent magnetization (IRM), and anhysteretic remanent magnetization (ARM) experiments were conducted on unshocked granitoid rocks and on impactites.

AF demagnetization results reveal distinct magnetic decay patterns among the lithologies. Unshocked rocks exhibit a peak in magnetization intensity at 10 mT, likely due to removal of a low-coercivity antiparallel component, followed by gradual decay, with median destructive field (MDF) values of ~20–60 mT and 65–90% loss of magnetization at 100 mT. Impact melt rocks exhibit smoother decay trends, with MDFs ranging from 10 to 40 mT, corresponding to 75–98% loss of magnetization at 100 mT. In contrast, monomict breccia displays the most unstable behavior with fluctuating magnetization intensity, often retaining >50% of remanence at 100 mT. The average mass-normalized saturation IRM1000mT values vary systematically among lithologies, with the lowest (4.18×10-3 Am2 kg-1) in monomict breccia, intermediate (1.11×10-2 Am2 kg-1) in impact melt rocks, and the highest (6.7×10-1 Am2 kg-1) in unshocked rocks. Average mass-normalized ARM values follow a similar trend, with the lowest (2.18×10-6 Am2 kg-1) in monomict breccia, intermediate (3.65×10-5 Am2 kg-1) in impact melt rocks, and the highest (1.03×10-2 Am2 kg-1) in unshocked rocks.

Together, these results demonstrate a progressive reduction in remanence acquisition capacity and magnetic stability from unshocked rocks to monomict breccia. Overall, the findings highlight that impact-generated shock waves significantly modify the domain state, coercivity spectrum, and remanence efficiency of the target rocks.

Reference: Pandey, A. K., Agarwal, A., Joshi, G., Sangode, S., & Venkateshwarlu, M. (2026). Shock demagnetization in an ambient magnetic field at the Dhala impact structure, India. Communications Earth & Environment. https://doi.org/10.1038/s43247-025-03164-6

How to cite: Pandey, A. K., Agarwal, A., Sangode, S. J., and Joshi, G.: Shock Effects on Magnetic Remanence in Rocks from the Dhala Impact Structure, India, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-587, https://doi.org/10.5194/egusphere-egu26-587, 2026.

EGU26-1428 | ECS | Orals | EMRP3.2

 Micromagnetic constraints on Pullaiah curves for magnetite 

Ualisson Donardelli Bellon, Wyn Williams, Lesleis Nagy, and Adrian R. Muxworthy

Fifty years ago, Pullaiah et. al (1975) derived temperature-dependent relaxation curves for single-domain (SD) magnetite, which have since been widely applied to a range of paleomagnetic problems. However, ideal SD behaviour is restricted to a narrow particle-size range. Most of the stable geological remanence carried by magnetite is instead held by vortex-state particles, for which SD theory fails to provide an adequate description. This study presents new numerical results for micromagnetically determined, temperature-dependent relaxation curves for submicron oblate, prolate and equidimensional cuboctahedral magnetite particles from 45-200 nm, with varying elongations. MERRILL was used to compute local energy-minimum (LEM) states over the full temperature range from 20 to 579 °C, and the nudged elastic band (NEB) method was employed to obtain energy barriers for use in Néel–Arrhenius estimates of relaxation times. The resulting relaxation curves are analysed and compared with the classical Pullaiah curves, highlighting the implications for interpreting paleomagnetic records carried by vortex-state particles.

How to cite: Donardelli Bellon, U., Williams, W., Nagy, L., and Muxworthy, A. R.:  Micromagnetic constraints on Pullaiah curves for magnetite, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1428, https://doi.org/10.5194/egusphere-egu26-1428, 2026.

EGU26-2019 | Orals | EMRP3.2

Identifying Framboidal Pyrrhotite: A Proxy for hydrothermal alteration of Organic-Rich Sediments 

Yong Zhang, Yin Wang, and Adrian Muxworthy

Framboidal pyrrhotite, in sharp contrast to framboidal pyrite, has been rarely reported, and its formation remains poorly understood. Here we report its clear identification in a shale‐gas well core and explore its potential as a proxy for diagenesis or low‐grade metamorphism of organic-rich sediments. A range of complementary results including petrography, geochemistry, rock magnetism and paleomagnetism, collectively support the identification of framboidal pyrrhotite, whose coexistence with other framboidal minerals indicates pseudomorphic replacement of framboidal pyrite. A strong correlation between total organic carbon and natural remanent magnetization, together with its restriction to organic-rich layers, highlights organic matter's role in its genesis. Paleomagnetic and vitrinite reflectance data further link its formation to magmatic heating (∼274°C). We therefore propose hydrothermal replacement of framboidal pyrite by framboidal pyrrhotite, involving heating and organic matter. This study highlights its diagnostic features, key conditions, and proxy potential for hydrothermal alteration and low‐grade metamorphism in organic-rich sediments.

How to cite: Zhang, Y., Wang, Y., and Muxworthy, A.: Identifying Framboidal Pyrrhotite: A Proxy for hydrothermal alteration of Organic-Rich Sediments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2019, https://doi.org/10.5194/egusphere-egu26-2019, 2026.

The Galápagos Archipelago has been formed as the Nazca Plate moved over a volcanic hotspot. The islands' age increases from west to east, and they exhibit pronounced climatic zonation, ranging from arid lowlands to humid highlands. In this work, topsoil and parent material samples from four islands, Isabela, Floreana, Santa Cruz, and San Cristóbal, were analyzed to investigate iron mineralogy as a function of island age and climate. Samples were collected from six sites in the humid highlands on all four islands, as well as from two sites in very dry and dry zones on Floreana and San Cristóbal, respectively.

Room-temperature Mössbauer spectroscopy and magnetic measurements, including hysteresis loops (up to 3.0 T) and temperature-dependent magnetization (50 – 1000 K), were performed to identify and characterize the iron-bearing phases. Mössbauer spectra reveal the presence of Fe²⁺ and Fe³⁺ doublets attributed to iron silicates, as well as a sextet corresponding to hematite. In all samples, the relative contribution of the Fe²⁺ doublet decreases from parent material to topsoil, accompanied by an increase in the Fe³⁺ doublet contribution. Samples from the older islands (Santa Cruz and San Cristóbal), in addition to the presence of Fe3+, showed an important sexted associated with hematite in the topsoil and parent material samples. We cannot rule out the contribution of fine particle size and superparamagnetic goethite and/or ferrihydrite associated with the Fe3+ doublet.

Climate-dependent variations are also evident. Mössbauer spectroscopy data of topsoil samples from humid environments exhibit a higher hematite contribution (59%) compared to those from dry environments (49%). For parent materials, humid conditions yield a 54% hematite contribution, whereas samples from dry conditions show a 17% contribution from maghemite. The magnetic results are complemented by hysteresis loops, which indicate the presence of a high-magnetization phase, consistent with Ti-magnetite and/or Ti-maghemite. The absence of a Verwey transition near 120 K in low-temperature magnetization curves and a drop in magnetization near 580 °C in high-temperature magnetization curves further support the presence of Ti-magnetite. AC magnetic susceptibility curves exhibit a frequency dependency, which may indicate a broad distribution of particle sizes, due to the contribution of superparamagnetic iron phases.

How to cite: Berquo, T. and Zehetner, F.: Magnetic investigation of iron oxides of the Galápagos Archipelago and the relationship with island age and climate, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4098, https://doi.org/10.5194/egusphere-egu26-4098, 2026.

EGU26-4440 | Orals | EMRP3.2

Microscale pseudo-Thellier palaeointensity using a Quantum Diamond Microscope 

Wyn Williams, Ualisson Bellon, Gelson de Souza-Junior, Adrian Muxworthy, Leonardo Uieda, Roger Fu, and Ricardo Trindade

In this study, we present the first full palaeointensity protocol based on quantum diamond microscope (QDM) measurements of the vertical magnetic field component (bz ) above thin sections of an archaeological ceramic. A key advantage of the QDM approach is that it enables the identification, isolation, and tracking of individual magnetic sources within a thin section, allowing ideal palaeomagnetic recorders to be analysed while excluding poorly behaved contributors that dominate bulk measurements. We invert magnetic moments associated with both near-surface and subsurface magnetic sources from QDM maps, and follow their response to alternating-field demagnetisation and anhysteretic remanent magnetisation (ARM) acquisition. Mean directions derived from these selectively inverted sources closely match bulk measurements obtained using a cryogenic rock magnetometer. We quantify the effects of filtering sources based on inversion quality and magnetic behaviour, and demonstrate that for well-separated dipole-like particles, pseudo-Arai slopes constructed from fitted ARM acquisition and AF demagnetisation curves yield palaeointensity estimates that agree, within uncertainty, with double-heating absolute palaeointensity determinations on sister samples. When combined with micro magnetic modelling constraints on the relationship between ARM and thermoremanent magnetisation, these results demonstrate that QDM-based palaeointensity methods offer a promising route toward high-precision, carrier-selective micropalaeomagnetic analysis at the thin-section scale.

How to cite: Williams, W., Bellon, U., de Souza-Junior, G., Muxworthy, A., Uieda, L., Fu, R., and Trindade, R.: Microscale pseudo-Thellier palaeointensity using a Quantum Diamond Microscope, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4440, https://doi.org/10.5194/egusphere-egu26-4440, 2026.

EGU26-4909 | Posters on site | EMRP3.2

Shallow Vertical Magnetic Susceptibility Profiles for Exploring Soil Discrimination across Multiple Locations Using Statistical and Geostatistical Methods 

Jaroslaw Zawadzki, Piotr Fabijańczyk, Michał Bućko, Hana Grison, Michał Jankowski, Tadeusz Magiera, Eduard Petrovsky, Vilém Podrázský, Marcin Sykuła, Marcin Szuszkiewicz, and Zdeněk Vacek

Magnetic susceptibility is a widely used non-destructive proxy for soil characterisation. In this study, shallow vertical magnetic susceptibility profiles were analysed to explore their potential for soil discrimination across multiple locations representing different environmental settings. Magnetic susceptibility was measured in situ down to a depth of 30 cm, providing high-resolution vertical profiles.

The analysis focused on vertical patterns and variability of magnetic susceptibility along the soil profile. A combination of descriptive statistics and geostatistical parameters, as well as multivariate analysis, was applied to assess similarities and differences among soil profiles from different locations. The applied methodology aimed to evaluate the reliability and applicability of magnetic susceptibility as a proxy for comparative soil analysis.

The results show that shallow vertical magnetic susceptibility profiles exhibit substantial variability among profiles and locations, allowing for the identification of characteristic vertical patterns and differences between locations. Geostatistical parameters provided additional insight into the spatial organisation of magnetic susceptibility along the vertical axis, supporting the interpretation of profile variability.

The study demonstrates that shallow vertical magnetic susceptibility profiles can support comparative analysis of soils across multiple locations, while also highlighting the limitations of using magnetic susceptibility alone for soil discrimination.

How to cite: Zawadzki, J., Fabijańczyk, P., Bućko, M., Grison, H., Jankowski, M., Magiera, T., Petrovsky, E., Podrázský, V., Sykuła, M., Szuszkiewicz, M., and Vacek, Z.: Shallow Vertical Magnetic Susceptibility Profiles for Exploring Soil Discrimination across Multiple Locations Using Statistical and Geostatistical Methods, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4909, https://doi.org/10.5194/egusphere-egu26-4909, 2026.

EGU26-4948 | Posters on site | EMRP3.2

Spatial Structure of Surface Soil Magnetic Susceptibility Measured with MS2D across Multiple Soil Types in Poland and the Czech Republic 

Piotr Fabijańczyk, Jarosław Zawadzki, Michał Bućko, Hana Grison, Michał Jankowski, Tadeusz Magiera, Eduard Petrovsky, Vilém Podrázský, Marcin Sykuła, Marcin Szuszkiewicz, and Zdeněk Vacek

This study examines the spatial variability of soil magnetic susceptibility measured on the soil surface across multiple sites in Poland and the Czech Republic. The investigated areas encompass a broad range of soil types, including Podzol, Gleysol enriched with iron ore, Rubic Arenosol, Ranker‑Cambisol, Cambisol, Luvisol, Brown acidic soil, and Podzolic brown soil. Surface magnetic susceptibility was measured with Bartington MS2D to capture both natural pedogenic patterns and potential anthropogenic magnetic enhancement. Spatial correlations were quantified using experimental variograms and their parameters to assess the scale and structure of spatial variability of soil magnetic susceptibility. Among these parameters, nugget effects varied substantially between soil types, indicating differences in micro-scale heterogeneity and surface disturbance.

The results demonstrate that surface magnetic susceptibility, combined with geostatistical analysis, is a sensitive indicator of both natural soil-forming processes and anthropogenic pollution.

How to cite: Fabijańczyk, P., Zawadzki, J., Bućko, M., Grison, H., Jankowski, M., Magiera, T., Petrovsky, E., Podrázský, V., Sykuła, M., Szuszkiewicz, M., and Vacek, Z.: Spatial Structure of Surface Soil Magnetic Susceptibility Measured with MS2D across Multiple Soil Types in Poland and the Czech Republic, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4948, https://doi.org/10.5194/egusphere-egu26-4948, 2026.

EGU26-5006 | Orals | EMRP3.2

The magnetic fabric of fine-grained sediments laid from the Cretan 365 CE tsunami on the SE coast of Sicily 

Leonardo Sagnotti, Alessandra Smedile, Paolo Marco De Martini, Raphaël Paris, and Christophe Lecuyer

Along Sicily's southeastern coast, sandy barriers and geological features isolate coastal lagoons known locally as "pantani." This study examines the anisotropy of magnetic susceptibility (AMS) in 69 oriented samples from the Pantano Morghella wetland, north of Portopalo. Collected in 2 cm³ plastic cubes from a single trench ~700 m from the present shoreline, samples follow two parallel profiles (alternated by 1 cm) spanning 134 cm of stratigraphic sequence. This includes sediments from one of antiquity's most devastating tsunamis, which struck offshore Crete on July 21, 365 CE (Gerardi et al., 2012, https://doi.org/10.5194/nhess-12-1185-2012).

The basal tsunami deposit at the trench site consists of a ca. 5 cm thick yellowish bioclastic sandy layer, whose abrupt and probably erosive lower boundary is at about 101.5 cm stratigraphic depth. The rest of the analysed stratigraphic sequence consists of massive grey to blackish muds and grey to pale brown muds, respectively below and above the tsunami sand.

Magnetic susceptibility profiles and AMS data divide the sequence into six zones, revealing distinct depositional environments.

Zone VI (134–101.5 cm): Lowest susceptibility (~500 × 10⁻⁶ SI) and oblate fabric, with a minimum susceptibility axis (kmin) close to the vertical and the maximum (kmax) and intermediate (kint) susceptibility axes scattered in the horizontal plane. This indicates undisturbed, low-energy lagoon/wetland deposition.

Zone V (101.5–94 cm): The sandy tsunami layer, with only three samples showing scattered AMS axes, reflecting chaotic high-energy deposition.

Zone IV (94–63 cm): High susceptibility (1000–2500 × 10⁻⁶ SI), prolate fabric, clustered E-W horizontal kmax, and kint and kmin axes scattered in the N-S vertical plane. This indicates deposition under the action of high-energy currents almost perpendicular to the coast.

Zone III (63–53 cm): Similar fabric to Zone IV but lower susceptibility, decreasing upward to ~500 × 10⁻⁶ SI, suggesting waning high-energy influence.

Zone II (53–35 cm): Returns to Zone VI-like low susceptibility and oblate fabric, typical of calm lagoon conditions.

Zone I (35 cm upward): High susceptibility (>2000 × 10⁻⁶ SI in top 20 cm) and triaxial fabric, linked to human salt pan activities – that started in the XIX century - altering sedimentation.

The trends of magnetic fabric are then compared to CT-scan data (X-ray microtomography) providing statistics of size, shape, and orientation of the sand grains. Overall, AMS analyses provide a robust proxy for paleoenvironmental reconstruction in Pantano Morghella. They distinguish intervals of undisturbed, low-energy sedimentation typical of a lagoon/wetland environment from those disrupted by natural catastrophes, such as the 365 CE tsunami, and later anthropogenic activities over the past two centuries.

How to cite: Sagnotti, L., Smedile, A., De Martini, P. M., Paris, R., and Lecuyer, C.: The magnetic fabric of fine-grained sediments laid from the Cretan 365 CE tsunami on the SE coast of Sicily, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5006, https://doi.org/10.5194/egusphere-egu26-5006, 2026.

In anoxic marine sediments, in steady state conditions, organoclastic sulfate reduction and anaerobic oxidation of methane release hydrogen sulfide to pore waters. Hydrogen sulfide, in turn, reacts with either solid-phase Fe(III) (oxyhydr)oxides or dissolved Fe2+ liberated by dissimilatory Fe(III) reduction to form iron sulfides with greigite as a precursor phase and pyrite as the end member of the reaction sequence. This process is characteristic for sulfate-methane transition zones (SMTZ). However, non-steady state conditions are common in marine sediments and the sequence described above may be disrupted. These conditions may lead to the preservation of early diagenetic greigite and/or to a late formation of greigite during burial enabled by reactivated biotic or abiotic processes. Site U1417 drilled during Integrated Ocean Drilling Program (IODP) Expedition 341 in the Gulf of Alaska has no shallow SMTZ and a deep inverse SMTZ at ~650 meters below sea floor, with a thick sulfate-free and methane-free zone above the deep inverse SMTZ, which makes non-steady state diagenetic conditions at this site unique. The deep inverse SMTZ is likely caused by tectonically-induced fluid circulation related to plate bending fractures. In this study, we aim to investigate how the inverse diagenetic zonation and related tectonically-induced fluid circulation impact the magnetic mineral assemblage and the paleomagnetic record in the sediment. We will pay special attention to the authigenic phases such as greigite which is responsible for secondary magnetizations. We will also assess the role of the diagenetic processes on the original detrital magnetic minerals, and their impact on the iron, sulfur, and carbon elemental cycles.

How to cite: Kars, M. and Zindorf, M.: Magnetic properties and mineralogy in non-steady state diagenetic conditions: Study in IODP Expedition 341 Site U1417 marine sediments, Gulf of Alaska, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5399, https://doi.org/10.5194/egusphere-egu26-5399, 2026.

EGU26-5424 | ECS | Posters on site | EMRP3.2

Magnetic Characterization of α-Fe Oxidation Kinetics: Implications for Source Attribution in Urban Pollution. 

Felix Ostermeier, Stuart Gilder, Nikolai Petersen, and Kai-Uwe Hess

Iron-bearing nano- and microparticles are ubiquitous in urban environments, often emitted by anthropogenic pollution sources. However, the occurrence of metallic iron (α-Fe) in non-reducing, near-surface environments is anomalous given the oxidizing nature of Earth’s atmosphere. Quantifying the magnetic changes associated with the oxidation kinetics of these particles allows for the determination of their atmospheric residence times. We conducted hysteresis measurements on synthetic iron powders of varying grain sizes (1-149 µm) at specific intervals following exposure to temperatures ranging from 200°C to 500°C. By plotting saturation magnetization (Ms), saturation remanent magnetization (Mrs), and coercive force (Hc) against oxidation time, we observed that oxidation is most likely diffusion-limited: it proceeds rapidly at the grain surface and decelerates as oxygen penetration becomes restricted by the oxide shell. Using MS decay as a proxy for oxidation progress, we constructed an Arrhenius plot to determine activation energies. This allows for the extrapolation of reaction rates to room temperature. Consequently, we present a method to estimate the time elapsed since particle emission. When combined with meteorological data, we can backtrack trajectories to pinpoint specific anthropogenic sources of α-Fe emission.

How to cite: Ostermeier, F., Gilder, S., Petersen, N., and Hess, K.-U.: Magnetic Characterization of α-Fe Oxidation Kinetics: Implications for Source Attribution in Urban Pollution., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5424, https://doi.org/10.5194/egusphere-egu26-5424, 2026.

EGU26-6469 | Orals | EMRP3.2

Relationship between surface-soil magnetic susceptibility and its shallow vertical distribution 

Eduard Petrovsky, Tadeusz Magiera, Michal Jankowski, Marcin Szuszkiewicz, Hana Grison, Marcin Sykula, Michal Bucko, Jarek Zawadzki, Piotr Fabijanczyk, and Sarka Stejskalova

Measurements of magnetic susceptibility on the soil surface are routinely used for, e.g., assessment of distribution of atmospherically deposited dust particles rich in iron oxides. In general, the data obtained using Bartington MS2D coil integrate signal from a depth down to about 10 cm, with non-linear response function. Therefore, it is believed that the iron oxides in this layer may be due to atmospheric deposition, weathering of lithogenic rocks, and pedogenic processes occurring directly in the soil. In order to assess the significance of these sources, as well as to observe the stratification of the soil column, shallow vertical soil cores, usually down to 30 cm, are used. However, there is no comprehensive comparison of the vertical distribution of magnetic susceptibility, projected on the surface, with the values actually measured on the soil surface. In our contribution, we use the known response function, defining the weight of magnetic susceptibility with depth, to obtain the total model susceptibility projected on the soil surface, and compare it with the real data measured in the field. Our results show that good agreement between the measured and modelled surface values is not a general rule. Thus, the use of shallow vertical distribution of susceptibility in terms of interpreting the data measured on the surface is subject to ambiguities and doubts.

How to cite: Petrovsky, E., Magiera, T., Jankowski, M., Szuszkiewicz, M., Grison, H., Sykula, M., Bucko, M., Zawadzki, J., Fabijanczyk, P., and Stejskalova, S.: Relationship between surface-soil magnetic susceptibility and its shallow vertical distribution, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6469, https://doi.org/10.5194/egusphere-egu26-6469, 2026.

EGU26-6858 | ECS | Posters on site | EMRP3.2

Towards nanometre-scale imaging of paleomagnetic recorders  

Silvi Klein Schiphorst, Philipp D’Astolfo, David Cortés-Ortuño, and Lennart de Groot

Quantum Diamond Microscopy (QDM) has opened new avenues for palaeomagnetism by enabling magnetic imaging at micrometre-scale spatial resolution, bridging the gap between bulk rock measurements and grain-scale magnetic observations. Micromagnetic Tomography (MMT) experiments integrate QDM data with micro- or nano-CT–derived grain geometries to determine magnetic moments of individual grains within a sample. Adding spatial information to the inversion problem makes it possible to calculate magnetic moments of individual iron-oxide grains even in samples with high grain concentrations, complex domain states, and overlapping magnetic signals. This enables the magnetic contribution of individual particles to be quantified, compared through consecutive (de)magnetization steps, and tested for stability. MMT therefore provides direct experimental access to grain-scale magnetic moments and goes beyond what bulk or surface-integrated measurements can reveal.

The goal of MMT has always been to isolate and select contributions of only the most reliable recorders in a rock sample. Nevertheless, MMT faces a fundamental challenge in spatial scales: wide-field QDM imaging achieves spatial resolutions of ~1 µm, while the practical resolution of micro- and nano-CT similarly limits the detection of magnetic particles to sizes of ~1 µm and larger. Magnetite and titanomagnetite grains in this size range are typically characterized by multidomain behaviour and are therefore often magnetically unstable, limiting their usefulness as reliable paleomagnetic recorders. As a result, current grain-scale approaches predominantly probe particles that are least suitable for preserving stable remanent magnetisations.

Accessing the information stored in smaller, submicron, vortex-state grains that are reliable recorders of the Earth’s magnetic field requires moving beyond wide-field QDM imaging. Improvements in spatial resolution of wide-field QDMs are fundamentally restricted by the optical diffraction limit, motivating a transition to Quantum Scanning Microscopy (QSM). In QSM, a single nitrogen-vacancy centre functions as an atomic-scale magnetometer, enabling nanometre-scale spatial resolutions that are ideal for magnetic imaging of vortex-state grains.

Here we present the first results of QSM stray-field imaging applied to a volcanic rock sample, in combination with slice-and-view FIB-SEM analysis of the same sample to characterise the particles’ geometries. These measurements demonstrate the feasibility of detecting magnetic signals at length scales inaccessible to wide-field QDM and current MMT techniques, while highlighting both the opportunities and technical challenges associated with pushing paleomagnetic observations into the nanoscale. Together, these developments provide a path forward towards resolving the magnetic behaviour of the particles that are most relevant for reliable paleomagnetic recording in rock samples.

How to cite: Klein Schiphorst, S., D’Astolfo, P., Cortés-Ortuño, D., and de Groot, L.: Towards nanometre-scale imaging of paleomagnetic recorders , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6858, https://doi.org/10.5194/egusphere-egu26-6858, 2026.

EGU26-8031 | Posters on site | EMRP3.2

Mapping Sources of Fine Metallic Particles Near Schools in Greater Paris Using Passive Biocaptors: transforming environmental monitoring practices 

Aude Isambert, Claire Carvallo, Laure Turcati, Yann Sivry, Gabriel Junghans, Eugénie Bontemps, Frédéric Fluteau, Nestor Herran, Justyna Moizard, and Christine Franke

As of 2024, 100% of Parisian residents remain exposed to concentrations of fine particulate matter (PM₂.₅) that exceed the World Health Organization’s (WHO) guideline limit of 5 µg/m³. Despite gradual improvements in air quality, atmospheric pollution—particularly from fine particles and nitrogen dioxide (NO₂)—continues to pose a major public health challenge. Recent findings by the French association Respire revealed that 682 daycare centers and schools in Île-de-France (Administrative region of Paris) exceed WHO NO₂ thresholds, underscoring the urgent need for intervention and the increasing mobilization of local stakeholders.

In the Paris region, wood heating and road traffic are the primary sources of fine particulate matter. Ultrafine particles (<1 µm), often enriched in heavy metals and exhibiting magnetic properties due to their iron content, present significant health risks. Their high reactivity and association with toxic metals suggest a potential link to neurodegenerative diseases.

This study presents the first results from the interdisciplinary Nanomap project (based on the Ecorc’Air scientific protocol), launched in 2024 in Île-de-France. The project integrates researchers from social sciences, geosciences, and participatory science, collaborating with nine citizen associations. Its objective is to map fine and ultrafine metallic particles pollution near schools and daycare centers, with the aim of tracing and determining the variability of pollution sources in urban areas. Additionally, the project examines scientific practices and interactions between researchers and citizen groups.

The study employs plane tree bark as a passive pollution sensor, leveraging its annual renewal and widespread presence in cities (more than 42,000 plane trees in Paris) to enhance spatial and temporal resolution. In 2025, nearly 700 samples were collected by citizens, with half of which were situated near educational facilities. Magnetic susceptibility measurements revealed varying concentrations of metallic particles.

Samples collected near potential pollution sources (e.g., ring roads, high-traffic areas) are currently undergoing advanced chemical analysis (ICP-MS and spICP-MS) and detailed magnetic characterization. This integrated approach is essential for validating suspected sources before any public disclosure to the citizen groups involved in the Nanomap project.

How to cite: Isambert, A., Carvallo, C., Turcati, L., Sivry, Y., Junghans, G., Bontemps, E., Fluteau, F., Herran, N., Moizard, J., and Franke, C.: Mapping Sources of Fine Metallic Particles Near Schools in Greater Paris Using Passive Biocaptors: transforming environmental monitoring practices, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8031, https://doi.org/10.5194/egusphere-egu26-8031, 2026.

Remagnetization in sedimentary basins is commonly regarded as “noise” that overprints primary remanence. However, if its acquisition timing and underlying mechanism can be constrained, remagnetization can instead be exploited as a physical archive of burial history, tectonic deformation, clay-mineral transformation, and hydrocarbon-related fluid activities. With the growing importance of hydrocarbon resource evaluation, magnetization resetting associated with organic-matter maturation and hydrocarbon migration has gradually become a major focus of remagnetization studies. To explore the relationship between remagnetization and hydrocarbon activity, we targeted the Upper Ordovician Zhaolaoyu Formation in the Fuping area along the southern margin of the Ordos Basin and carried out an integrated investigation combining petrographic observations, rock-magnetic experiments, paleomagnetic analyses, and organic geochemical measurements.

The results showed that magnetite was the dominant magnetic carrier, and stepwise demagnetization isolated a stable characteristic remanent magnetization. The corresponding paleomagnetic pole matched the Early–Middle Triassic segment of the apparent polar wander path of the North China Block, indicating a Triassic remagnetization. Anisotropy of magnetic susceptibility results indicated a primary sedimentary compaction fabric, and together with previous high-resolution Sr-isotope studies showing no signature of tectonically derived fluids in the section, these observations effectively ruled out remagnetization driven by subsequent tectonic fluids. Optical microscopy showed heterogeneous iron-oxide infillings within microfractures, and SEM further revealed spherical magnetite developed within microfractures; fluorescence microscopy also indicated that organic matter was predominantly hosted within microfractures. Collectively, these microscopic observations suggested that the spatial distribution of authigenic magnetite may be linked to the presence of organic matter. Notably, based on the commonly used parameter (NRM–TOC), natural remanent magnetization (NRM) showed a significant positive correlation with total organic carbon (TOC), further supporting an association between remagnetization in the Zhaolaoyu Formation and hydrocarbon activity. Meanwhile, we introduced the hydrocarbon generation potential (Pg) and the ratio of effective specimen number to total specimen number (N₀/N), and established quantitative relationships between Pg and NRM, as well as between N₀/N and TOC to evaluate the relationship between magnetic records and organic matter. Both relationships showed positive correlations.

In summary, the Zhaolaoyu Formation records an Early–Middle Triassic chemical remagnetization event associated with organic-matter maturation. This interpretation is consistent with previous hydrocarbon-generation modeling results for the study area. This study provides key constraints on the hydrocarbon-generation evolution of Ordovician source rocks along the southern margin of the Ordos Basin and, for the first time in the Ordos Basin, verifies the feasibility and applicability of using remagnetization as a tool to constrain hydrocarbon activity. In addition, the two parameter sets proposed in this study (NRM–Pg and N0/N–TOC) provide new quantitative metrics that can be applied to explore similar remagnetization mechanisms in other stratigraphic intervals and sedimentary basins.

How to cite: Lan, S., Cheng, X., and Wu, H.: Hydrocarbon-linked chemical remagnetization in the Upper Ordovician Zhaolaoyu Formation, southern margin of the Ordos Basin: constraints from paleomagnetism and geochemistry, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8962, https://doi.org/10.5194/egusphere-egu26-8962, 2026.

EGU26-10591 | Orals | EMRP3.2

Towards Thermally Activated High-Field Micromagnetism 

Greig Paterson, Brendan Cych, Lesleis Nagy, and Wyn Williams

High-field magnetic measurements and procedures, such as hysteresis, first-order reversal curves (FORC), and alternating-field (AF) demagnetization, are foundational methods in rock and paleomagnetic studies. Interpreting these data can be challenging and often requires an understanding of the particle scale contributions to these signals. This requires a numerical approach using micromagnetic models along with the inclusion of thermal fluctuations, which result in time dependent relaxation in experimental observations. This is a challenge that requires knowledge of all stable domain states, their connectivity, and  energy barriers that partition the energy landscape that results from the field strength and orientation of each particle. This typically requires considerable user input and analysis, making this an unfeasibly time-consuming endeavor.

We are developing a method that calculates exact energy surfaces for uniformly magnetized particles and approximate energy surfaces for single vortex (SV) particles, akin, to software tools such as the Singe Domain Comprehensive Calculator (SDCC; Cych et al., 2025, doi: 10.1093/gji/ggaf149). This technique is integrated into the micromagnetic software package MERRILL and readily identifies minimum energy domain states, their connectivity, and (using the nudged elastic band method), can calculate the energy barriers between states. This automated process dramatically reduces user input and analysis at the cost of additional computational time resulting in high-field energy landscapes (HELs) which can then be used to simulate a wide range of thermally activated experiments, including hysteresis loops, FORC diagrams, anhysterestic remanent magnetization (ARM) acquisition and AF demagnetization. Additional computational resources are not, however, significant, since our method runs in a matter of minutes to hours on a modern laptop computer. This new approach will take the rock and paleomagnetic community one step closer to incorporating micromagnetic tools as a part of the standard analytical repertoire used to interpret the behavior of natural samples and reconstruct the signals they carry.

How to cite: Paterson, G., Cych, B., Nagy, L., and Williams, W.: Towards Thermally Activated High-Field Micromagnetism, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10591, https://doi.org/10.5194/egusphere-egu26-10591, 2026.

First-order reversal curves (FORC) are gaining increasing popularity as an effective tool for characterizing magnetic minerals in rocks and sediments. The associated two-dimensional representation of hysteretic magnetization processes, known as FORC diagrams, enables the identification of specific fingerprints associated with magnetic grain size and mineralogy, and, in certain cases, the separation of magnetic components with widely overlapping coercivities, thus reducing the ambiguity of other magnetic characterization techniques. Recent progress in micromagnetic calculations also enable to calculate FORC diagrams for given magnetic mineral assemblages with enough statistical relevance to enable direct comparisons with real counterparts. Yet, interpretation ambiguities cannot be totally excluded, due to the different magnetization processes underlying each point of the FORC diagram. The additional measurement of zero-field hysteresis measurements to the original measurement protocol (Zhao et al., 2017) enables the separation of reversible and irreversible magnetization processes on a non-local basis, yielding different types of diagrams for each contribution. A local solution, which works for every point along a magnetization curve, is proposed here. It consists in the repeated measurement of Rayleigh loops in the applied field of the classic FORC protocol, as if low-field susceptibility would be instantaneously measured on the top of magnetometric measurements. Adequate processing of this modified measurement protocols divides the slope of magnetization curves into four contributions originating from (1) irreversible, (2) reversible, (3) viscous, and (4) aftereffect magnetization processes. Selected examples show the additional information that can be extracted from these measurements, as well as the disambiguation of not yet explained FORC features associated with the pseudo-single-domain and multidomain signatures of magnetite particles.

How to cite: Egli, R.: FORC-Rayleigh: A new measurement protocol for investigating the origin of magnetization changes in first-order reversal curves, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11730, https://doi.org/10.5194/egusphere-egu26-11730, 2026.

EGU26-12388 | Posters on site | EMRP3.2

New results of the Ecorc’Air citizen science project: Biomonitoring of Vehicular Air Pollution in Cologne, Germany 

Christine Franke, Stephanie Scheidt, Claire Carvallo, Aude Isambert, Kathrin Jung, Yann Sivry, and Laure Turcati

Airborne particulate matter (PM) is known to have serious effects on human health. Unfortunately, assessing spatial variability of PM at high resolution remains challenging due to limitations in the number of existing regulatory air quality stations in cities. As an alternative approach, biomonitoring using vegetation within cities has been proposed in recent years.

In the framework of the Ecorc’Air citizen science project, a robust protocol has been developed based on the annual collection of plane tree bark, which serves as a passive airborne PM collector using magnetic susceptibility as a proxy parameter to estimate PM abundance in cities (Carvallo et al. 2024). This has been used to create annual maps showing the variations in magnetic particle concentrations. Since the project started in Paris (France) in 2016, there has been a growing participation of inhabitants, associations, and municipalities and it has recently grown beyond national borders.

In Germany, sampling took place downtown Cologne in spring 2025 as part of the DFG-funded project “Mapping the concentration of particles in the air in the city of Cologne using environmental magnetic techniques – a first step towards participation in the European science network Euro'Air”. In this presentation, we focus on the results obtained from analyzing the collected plane bark samples. We show the spatial distribution of magnetic susceptibility and frequence dependent magnetic susceptibility. Additionally, our preliminary results from attempts to characterize the particles by magnetic hysteresis parameters and first order reversal curves (FORC) as well as scanning electron microscopy (SEM/EDX) analyses. The outcome will be discussed with respect to the spatial distribution of the PM concentrations in Cologne.

How to cite: Franke, C., Scheidt, S., Carvallo, C., Isambert, A., Jung, K., Sivry, Y., and Turcati, L.: New results of the Ecorc’Air citizen science project: Biomonitoring of Vehicular Air Pollution in Cologne, Germany, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12388, https://doi.org/10.5194/egusphere-egu26-12388, 2026.

EGU26-13427 | Posters on site | EMRP3.2

On the precision of anisotropy of magnetic remanence: Measuring designs, high-field experiments and tensor fitting toolbox 

Martin Chadima, František Hrouda, and Josef Ježek

Unlike anisotropy of magnetic susceptibility (AMS), which can be determined in a more or less simple way, the determination of anisotropy of magnetic remanence (AMR) is a relatively complex and laborious procedure involving a series of demagnetizations, directional magnetizations and measurements of the imparted directional remanence.

This complexity may logically imply larger errors in subsequent fitting of the AMR tensors compared to the AMS. The accuracy of the AMR determination primarily depends on the precision of imparting the directional remanence, the number of measuring directions, and the symmetry of the measuring design. The importance of the above control factors was investigated by means of mathematical modelling.

As shown in the previous model studies, the precision of the determination of the anisotropy of magnetic remanence (AMR) is directly proportional to the precision of the determination of the directional remanent magnetizations with respect to the degree of anisotropy. While the AMR imparted in weak to moderate fields is relatively commonly used in rock fabric studies (e.g., anisotropy of anhysteretic remanent magnetization), only a few attempts to determine the AMR in high fields (hfAMR) were reported most likely due to instrumental (insufficient precision in setting up the intensity of magnetizing field and its insufficiently homogeneity) or other methodological reasons.

Recently, a high-field impulse magnetizer has been developed (commercial name PUMA) that allows the standard palaeomagnetic specimen to be magnetized in a set of 18 predefined directions in the wide range of magnetic fields ranging from 1 mT to 5 T.

The elaborate design of this magnetizer allows precise setting of the pulse intensity and high homogeneity of the field over the entire specimen volume. To experimentally assess the precision of the hfAMR determination, the reproducibility in imparting the magnetic remanence in the same direction by the same magnetizing field was examined. We also investigated whether it was necessary to demagnetize the specimen between individual magnetizations to improve the remanence reproducibility despite the fact that each high field magnetization (“saturation”) should theoretically obliterate the previous remanence. The investigations were made on specimens having single mineral ferromagnetic fraction (magnetite, hematite, and pyrrhotite). The results helped us to decide whether the hfAMR is convenient to most rocks or only to strongly magnetic and strongly anisotropic ones.

In order to fit the AMR tensors, we present a simple, user-friendly toolbox which facilitates tensor fitting from an array of magnetic remanence vectors according the chosen magnetizing design (6, 9, 12, 15, 18 directions). This toolbox provides a graphical visualization of the intensity of measured remanence vectors and their directional comparison with the respective magnetizing directions.

How to cite: Chadima, M., Hrouda, F., and Ježek, J.: On the precision of anisotropy of magnetic remanence: Measuring designs, high-field experiments and tensor fitting toolbox, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13427, https://doi.org/10.5194/egusphere-egu26-13427, 2026.

EGU26-13503 | Orals | EMRP3.2

Quantitative relationship between opAMS and ipAMS in some pyrrhotite-bearing rocks 

Frantisek Hrouda, Martin Chadima, and Josef Ježek

The anisotropy of magnetic susceptibility (AMS) of pyrrhotite-bearing rocks (typically represented by ultramafic rocks) is often composite, carried not only by pyrrhotite, but also by magnetite and mafic silicates. In magnetic fabric studies, it is therefore desirable to separate the AMS component due to pyrrhotite from that due to the rest of the rock. This can be made, in addition to other techniques, by the anisotropy of the out-of-phase component of the AMS (opAMS). For comparative studies, it is vital to know quantitative relationship between opAMS and ipAMS, which is the aim of this paper. This knowledge is useful in interpreting the AMS of rocks in which pyrrhotite is important but not dominant magnetism carrier.

The out-of-phase susceptibility (opMS) of the pyrrhotite-bearing rocks investigated increases significantly with the field intensity within the field range between 10 A/m and 700 A/m. The increase is faster in very low fields (<100 A/m) than in stronger fields. The principal directions of the opAMS are virtually field independent in the entire low-field range used, being also very well parallel to the ipAMS directions. The degree of opAMS is also virtually field independent, but much higher than the degree of ipAMS. The shape parameter in opAMS is also field independent and resembles that in ipAMS.

The Rayleigh Law range, in which magnetization is linearly related to the field, is relatively narrow, less than 40 A/m. Theoretical quadratic relationship was suggested by Markert and Lehman (1996, GJI) between the tensor of initial ipMS and the tensor of Rayleigh coefficient characterizing the opAMS. The tensors are related by a constant c, which in general may or may not be direction independent. The direction independence would give rise to very simple relationship between the respective anisotropy degrees. Our investigations show that the constant c is in case of pyrrhotite direction independent. The tensor of the Rayleigh coefficient can be calculated from the opAMS measurement in one field, while the same tensor determined from field variation of ipAMS requires measurement in multiple fields (in two in minimum).

How to cite: Hrouda, F., Chadima, M., and Ježek, J.: Quantitative relationship between opAMS and ipAMS in some pyrrhotite-bearing rocks, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13503, https://doi.org/10.5194/egusphere-egu26-13503, 2026.

EGU26-13582 | Posters on site | EMRP3.2 | Highlight

Rock magnetic and microstructural investigation of Fe-bearing coatings on sand grains from the Namib Sand Sea 

Julie Carlut, Laurie Barrier, Lucie Perrenx, and Oscar Bruneau

The Namib Desert (Namibia) hosts giant dune fields whose sand color ranges from yellow to deep red. While provenance and grain composition contribute to these variations, a major control is the occurrence of Fe-bearing coatings (“varnish”) made of iron oxides and oxyhydroxides (e.g., magnetite, hematite, goethite) that surround sand grains. In this study, we analyze a set of 10 samples collected across various environments within a ~600 km perimeter in the northern Namib Desert. The mineralogical and textural nature of these coatings was investigated using a rock-magnetic approach. We combine bulk magnetic measurements, including magnetic susceptibility, hysteresis parameters, IRM acquisition, and thermomagnetic experiments, to identify the dominant magnetic carriers and assess the relative contributions of ferrimagnetic versus antiferromagnetic phases. These data are coupled with complementary mineralogical analyses (optical and scanning microscopy, Raman spectroscopy). Preliminary observations suggest that the magnetic phases are embedded in a clay-rich matrix and may be associated with microbial aggregates, raising questions about their origin and formation pathways. Furthermore, dune, terrace, and riverbed samples display distinct magnetic signatures, indicating the role of transport and/or in situ processes. By linking magnetic signatures to colorimetric variability and microstructural observations, this study aims to evaluate sand color as a potential environmental proxy for sediment transport pathways, weathering conditions, and hydroclimatic controls on iron oxide formation in arid environments.

How to cite: Carlut, J., Barrier, L., Perrenx, L., and Bruneau, O.: Rock magnetic and microstructural investigation of Fe-bearing coatings on sand grains from the Namib Sand Sea, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13582, https://doi.org/10.5194/egusphere-egu26-13582, 2026.

EGU26-16059 | Orals | EMRP3.2

Absolute Paleointensity Through Quantum Diamond Microscope Measurements 

Gelson F. Souza-Junior, Leonardo Uieda, Ricardo I. F. Trindade, Ualisson D. Bellon, Carolina S. de Moraes, and Roger Fu

Absolute paleointensity reconstructions provide critical constraints on the dynamics and long-term evolution of the geodynamo. Yet, a high failure rate persists in paleointensity experiments due to limitations inherent to bulk measurement techniques. As a result, measurements are often compromised by mineralogical alteration, multidomain behavior, magnetic interactions, and the presence of non-ideal remanence carriers that cannot be spatially isolated or individually evaluated. We present a new approach to absolute paleointensity determination based on Quantum Diamond Microscopy (QDM), enabling direct observation of thermoremanent magnetization (TRM) acquisition and decay at the sub-millimeter scale. We apply this technique to natural basalt and archaeological ceramic samples subjected to controlled laboratory TRM inductions, providing an opportunity to investigate magnetic recording processes at the level of localized anomalies. Experimental tests of TRM acquisition demonstrate that the direction of the applied laboratory field can be recovered from the magnetic vectors obtained from several hundred individual anomalies. For bias fields exceeding 2μT, the recovered vectors closely match the bulk direction, with minimal angular misfits across the population of carriers. This result provides direct physical validation, at the grain scale, of fundamental paleomagnetic recording assumptions that are traditionally inferred from statistical behavior in bulk measurements. This directional fidelity establishes the physical basis for extending micro-scale observations to quantitative paleointensity analysis. Using QDM, we implemented a full Thellier-style zero-field/in-field (ZI) protocol, monitoring both the thermal decay of natural remanent magnetization (NRM) and the acquisition of partial TRM (pTRM) on an anomaly-by-anomaly basis. This allows the identification and isolation of ideal magnetic recorders while excluding poorly behaving carriers, and enables the construction of localized Arai diagrams with a level of selection and quality assessment unattainable in conventional bulk techniques. The ceramic sample shows highly consistent paleointensity estimates, highlighting the robustness of the method. In contrast, paleointensity estimates for the basalt sample show larger variability, reflecting the influence of non-ideal magnetic carriers and local mineralogical heterogeneity. However, when rigorous spatial quality criteria are applied, including high Arai diagram linearity and vectorial decay constraints, the resulting paleointensity estimates converge toward the laboratory field with substantially improved accuracy and reduced uncertainty compared to bulk magnetometer results. Our results demonstrate that absolute paleointensity can be reliably determined at the micro-scale through the controlled ensemble analysis of magnetic anomalies. This approach represents a significant methodological advance in paleomagnetism, opening new perspectives for high-precision paleointensity studies of magnetically heterogeneous, minute, or rare materials, including meteorites, archaeological artifacts, and single crystals.

How to cite: F. Souza-Junior, G., Uieda, L., I. F. Trindade, R., D. Bellon, U., S. de Moraes, C., and Fu, R.: Absolute Paleointensity Through Quantum Diamond Microscope Measurements, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16059, https://doi.org/10.5194/egusphere-egu26-16059, 2026.

EGU26-2876 | ECS | Orals | EMRP3.3

Regional archeointensity curve from 600 BCE to 1700 CE for East Asia and possible recurrence of the weak field intensity 

Yutaka Yoshimura, Hyeon-Seon Ahn, Chie Kato, Yuhji Yamamoto, Chisato Anai, Yoshinori Tajiri, Tadahiro Hatakeyama, and Masao Ohno

In recent years, there have been reports suggesting the possibility of the West Pacific Anomaly existing in East Asia during the 16th century. To verify whether the anomaly existed in other ages, reliable archeomagnetic intensity (archeointensity) measurements from fired archeological materials in East Asia are necessary. Therefore, we conducted a study on archeointensity and rock magnetism using several Japanese pottery fragments from the Yayoi period, which were made in three stages. Thermomagnetic analysis revealed that the induced magnetization curve in air was more reversible than that in vacuum. Based on these results, we conducted the Tsunakawa-Shaw method with heating in air. As a result, we obtained archeointensities from 18 out of 20 specimens belonging to 4 out of 6 pottery fragments, which were made in three stages. When the average values of the three stages are arranged in chronological order, from 250 BCE to 50 BCE, the archeointensity remained nearly constant at 39.4 ± 4.2 µT to 38.6 ± 5.0 µT, and from 50 BCE to 50 CE, an increase in archeointensity was observed, from 38.6 ± 5.0 µT to 46.8 ± 2.0 µT. We constructed a reference curve from -530 CE to 1725 CE using a total of 30 archeointensity data from the present study and recent studies in Japan and South Korea. In this reference curve, two minima and two maxima were observed. Among these, we newly discovered a minimum around 150 BCE. The time intervals between the minimum and minimum, as well as between the maximum and maximum, were both approximately 900 years. Besides, this suggests the possibility that the West Pacific Anomaly occurred in East Asia at approximately 900-year intervals. This indicates that the reversed flux patch that causes the West Pacific Anomaly may recur at intervals of ~900 years at the core-mantle boundary near East Asia. The characteristic time-interval of approximately 900 years is similar to the recurrence time-interval of the South Atlantic Anomaly, which implies that the common cause (e.g., planetary gyre) may modulate both anomalies.

How to cite: Yoshimura, Y., Ahn, H.-S., Kato, C., Yamamoto, Y., Anai, C., Tajiri, Y., Hatakeyama, T., and Ohno, M.: Regional archeointensity curve from 600 BCE to 1700 CE for East Asia and possible recurrence of the weak field intensity, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2876, https://doi.org/10.5194/egusphere-egu26-2876, 2026.

EGU26-6999 | ECS | Posters on site | EMRP3.3

PyRotate: An automated framework for the analysis, visualisation, and interpretation of tectonic rotations using palaeomagnetic data 

Oliver Ross, Bruno Leite Mendes, Bram Vaes, and Daniel Pastor-Galán

Palaeomagnetic measurements provide the most robust, quantitative constraints on vertical axis rotations from outcrop scale blocks to entire tectonic plates. Vertical axis rotations are typically shown on maps as vectors representing local palaeodeclinations or individual rotations to a reference at the site level. When dealing with large and noisy datasets, however, this approach struggles to pick out underlying spatial patterns or finer scale regional displacements, especially when the data has variable density across regions.

These limitations are compounded in areas where several rotations events have been recorded across multiple scales or are poorly recorded in the palaeomagnetic record. As a result, both the visualisation and interpretation of complex rotation fields are hindered.

Here, we introduce PyRotate: a robust and scalable, end-to-end workflow for integrating and analyzing locality-level palaeomagnetic data from multiple sources. This framework allows users to curate and clean data through custom parameters, and to apply bootstrap techniques to determine the rotation of selected blocks and plates. Novel tools include kriging of rotations by age to simplify areas of highly variable rotation amounts and estimate interpolations between sites, giving an overlain interpolated rotation field as a visualisation tool, as well as automated outlier detection and labelling through cluster analysis. In addition, outputs are compatible with both PmagPy (Tauxe et al., 2016) and PyGPlates (Mather et al., 2024) as the basis of further analysis.

To illustrate the capabilities of PyRotate, we analyse a curated paleomagnetic dataset from Japan, and multiple-source datasets directly obtained from the Magic database. This analysis tests the ability of the workflow to deal with noisy and unevenly distributed datapoints. The tools introduced in PyRotate enable easier identification of areas needing additional sampling, synthesis of disparate datasets, and interpretation of the rotation of blocks through time.

How to cite: Ross, O., Leite Mendes, B., Vaes, B., and Pastor-Galán, D.: PyRotate: An automated framework for the analysis, visualisation, and interpretation of tectonic rotations using palaeomagnetic data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6999, https://doi.org/10.5194/egusphere-egu26-6999, 2026.

EGU26-7190 | Posters on site | EMRP3.3

Towards a regional Late Pleistocene and Holocene Paleomagnetic Secular Variation stack for the Tibetan Plateau 

Santiago Otero, Junbo Wang, Liping Zhu, Qingfeng Ma, Jiangting Ju, Andrew Henderson, Leon Clarke, Marie-Luise Adolph, Hendrik Vogel, Guillaume St-Onge, and Torsten Haberzettl

High-altitude lakes on the Tibetan Plateau preserve sensitive records of hydroclimate and atmospheric circulation, but establishing robust chronologies is often hindered by core-recovery artifacts, section-to-section discontinuities, and uncertainties in radiocarbon dating. Here we present a paired paleomagnetic strategy based on sediment cores from two high-altitude Tibetan lakes, Taro Co and Nam Co, to develop reproducible geomagnetic tie points for inter-core and inter-basin correlation.

For Taro Co (31°07′53.89″N, 84°07′50.65″E; ~4,566 m a.s.l; ~474 km²; max depth 130 m; catchment ~7,423 km²), we target two 8 m long parallel sediment cores spanning ~25 kyr. In parallel, we apply the same workflow to sediments recovered by the ICDP NamCore project from the central basin of Nam Co (30°30′–30°56′N, 90°16′–91°03′E,~4,718 m a.s.l.,~2,017 km², catchment ~10,680 km²,max depth ~99 m), enabling a comparison between independent sedimentary archives from the Tibetan Plateau.

We perform stepwise alternating-field demagnetization of the natural remanent magnetization (NRM) and determine characteristic remanent magnetization (ChRM) directions using principal component analysis (PCA). The datasets include inclination, relative declination, maximum angular deviation (MAD), and median destructive field (MDF), measured at 1 cm stratigraphic resolution. A key methodological focus is quality control across core sections and overlaps in both records: we assess directional stability and evaluate consistency between overlapping intervals to maximize recovery of the paleomagnetic secular variation (PSV) signal. Initial results from Taro Co show strong agreement in inclination between the two parallel cores, supporting the reproducibility of the PSV signal across holes.

The resulting PSV curves from Taro Co and Nam Co provide an independent stratigraphic framework to (i) test and refine radiocarbon-based chronologies, (ii) strengthen correlations between parallel holes/sections within each lake, and (iii) identify shared directional highs and lows between lakes. Ultimately, our goal is to build a preliminary inter-lake PSV stack for the SW/central Tibetan Plateau, improving regional synchronization and helping separate geomagnetic variability from site-specific recording effects.

 

 

How to cite: Otero, S., Wang, J., Zhu, L., Ma, Q., Ju, J., Henderson, A., Clarke, L., Adolph, M.-L., Vogel, H., St-Onge, G., and Haberzettl, T.: Towards a regional Late Pleistocene and Holocene Paleomagnetic Secular Variation stack for the Tibetan Plateau, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7190, https://doi.org/10.5194/egusphere-egu26-7190, 2026.

EGU26-8220 | Posters on site | EMRP3.3

Secular variation of the geomagnetic field in Sub-Saharan Africa over the last millennia: new archaeomagnetic data from West Africa and Ethiopia. 

Gwenael Hervé, Lamya Khalidi, Caroline Robion-Brunner, Vincent Serneels, Aurélie van Toer, Camille Wandres, Lebarama Bakrobena, Emmanuelle Delqué-Kolic, Pakou Harena, Julien Mantenant, Anne Mayor, Didier N'Dah, Giorgia Ricci, and Alexander Walmsley

Instrumental observations highlight that intertropical Africa is one of the areas with the most rapid changes in the modern geomagnetic field. The secular variation beyond the last centuries is poorly known due to lack of data, this large region representing only 0.7% of the GEOMAGIA50 database. The resulting large uncertainties in global geomagnetic models in this area make in particular the history of the present South Atlantic anomaly unclear. Here, we present archaeomagnetic studies in Southern Benin, Northern Togo, Eastern Senegal and Northeastern Ethiopia. In order to study the full geomagnetic vector, most fieldworks focus on in-situ archaeological structures sampled using the plaster cap technique, one oven in Ethiopia (mid 2nd mill. BCE), 11 iron furnaces in Senegal (500 BCE – 800 CE), 5 iron furnaces in Benin (13-15th c. CE) and 7 iron furnaces in Togo (18-20th c. CE). In Benin, we also sampled displaced baked clays associated to iron metallurgy (kiln walls, tuyeres, potteries).

Archaeodirections were determined after thermal demagnetization. We obtained 13 average directions, one in Ethiopia, 5 in Benin and 7 in Togo). The Senegalese structures provided scattered directions, probably because of tilting of the structure walls after the last heating. Archaeointensities were acquired using the classical Thellier-Thellier protocol with anisotropy and cooling rate corrections. The relatively high success rate (75% on average) allowed us to obtain 21 new average data, one on the Ethiopian oven, ten on the Beninese furnaces, 7 on the Togolese ones and 3 preliminary data on the Senegalese structures. The most recent 19-20th c. CE data from Togo are in very good agreement with the local predictions of the geomagnetic global models. At earlier periods, the new data are in agreement with, if any, already published data as in the 13-15th c. CE in West Africa. They highlight faster changes than the models, highlighting their importance to improve our knowledge of the secular variation of the geomagnetic field over the last 4 millennia.

How to cite: Hervé, G., Khalidi, L., Robion-Brunner, C., Serneels, V., van Toer, A., Wandres, C., Bakrobena, L., Delqué-Kolic, E., Harena, P., Mantenant, J., Mayor, A., N'Dah, D., Ricci, G., and Walmsley, A.: Secular variation of the geomagnetic field in Sub-Saharan Africa over the last millennia: new archaeomagnetic data from West Africa and Ethiopia., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8220, https://doi.org/10.5194/egusphere-egu26-8220, 2026.

EGU26-10115 | Posters on site | EMRP3.3

Iron Age Geomagnetic Intensity Variations in the Eastern Mediterranean: New Evidence from Cyprus 

Evdokia Tema, Juan Morales, Avto Goguitchaichvili, and Pamela Gaber

The strategic geographical position of Cyprus at the crossroads of civilizations in the eastern Mediterranean provides a unique opportunity to investigate past geomagnetic field variations and to fill the spatial gap between Eastern Europe and the Levant. In this study, we present new archaeointensity data obtained from well-dated ceramic assemblages from the ancient Kingdom of Idalion, one of the most significant archaeological sites on the island. A comprehensive palaeomagnetic and rock magnetic investigation, combined with Thellier-type experiments modified after Coe, was conducted to assess the magnetic mineralogy, thermal stability, and reliability of the remanent magnetization carried by the pottery sherds. A total of 186 specimens from 55 independent ceramic fragments were analyzed, and reliable archaeointensity estimates were obtained after correction for magnetic anisotropy and cooling-rate effects. The resulting field intensity values range between 50 and 80 µT, providing evidence for the occurrence of significant and rapid geomagnetic field variations in the eastern Mediterranean during the early first millennium BCE. These results are consistent with the Levantine Iron Age Anomaly (LIAA), previously documented in the Middle East. Our new data demonstrate the key role of Cypriot ceramics in constraining the spatial and temporal evolution of the LIAA and contribute to a more detailed regional reconstruction of geomagnetic secular variation. Furthermore, the pronounced and rapid intensity fluctuations recorded during the Iron Age highlight the potential of archaeomagnetic intensity as a robust dating tool for ceramic materials, offering a valuable alternative in periods affected by the Hallstatt radiocarbon plateau.

How to cite: Tema, E., Morales, J., Goguitchaichvili, A., and Gaber, P.: Iron Age Geomagnetic Intensity Variations in the Eastern Mediterranean: New Evidence from Cyprus, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10115, https://doi.org/10.5194/egusphere-egu26-10115, 2026.

EGU26-10782 | ECS | Posters on site | EMRP3.3

First Global Paleomagnetic model including the Gauss-Matuyama reversal 

Pablo Rivera, Monika Korte, Ahmed Mahgoub, Sanja Panovska, and Sunaina Shinu

Polarity reversals are among the most relevant events in Earth’s magnetic field evolution and are crucial to understand the dynamics within the outer core. During a reversal, the geomagnetic field deviates from an axial dipole, with non-dipolar components becoming dominant and resulting in a more complex spatial geometry. Therefore, paleomagnetic models based on Spherical Harmonic Analysis (SHA) have become an essential tool for analyzing the spatial and temporal features of the geomagnetic field during these events. However, to date, only the most recent magnetic field reversal, the Matuyama-Brunhes (MB) reversal (780 kyr BP), has been modeled.

Here we present and discuss our first SHA model of the second most recent reversal, the Gauss-Matuyama (GM), constructed from a recent compilation of high-quality paleomagnetic sediment records spanning from 2.4 to 2.7 Myr BP . Our model is based on 19 sediment cores, that have been carefully checked for independent age information, data quality and, where possible, regional consistency of the records. This provides a global distribution that allows us to analyze the spatial and temporal geometry of the GM worldwide. We further compare the field characteristics during the GM reversal to those of the MB reversal and to the present-day field. We discuss similarities and differences between the two geomagnetic field reversals.

 

How to cite: Rivera, P., Korte, M., Mahgoub, A., Panovska, S., and Shinu, S.: First Global Paleomagnetic model including the Gauss-Matuyama reversal, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10782, https://doi.org/10.5194/egusphere-egu26-10782, 2026.

EGU26-11365 | Posters on site | EMRP3.3

Paleomagnetic variations along the Southern Coast of Brazil from 46.06-5.36 ka BP using a Gaussian Process Technique 

Everton Frigo, Ítalo Gomes Gonçalves, Jairo Francisco Savian, Jaime Yesid Suárez-Ibarra, Sanja Panovska, Gelvam André Hartmann, Caroline Azzolini Pontel, Camila Trindade Lopes, María Alejandra Gómez Pivel, João Carlos Coimbra, Sandro Monticelli Petró, Adriana Leonhardt, and Ricardo Ivan Ferreira da Trindade

Understanding geomagnetic variations observed at the Earth’s surface requires knowledge of processes occurring in the Earth’s interior that are associated with the geodynamo. Because these processes occur at inaccessible depths, numerical models are used to simulate the expected conditions within these regions. On the other hand, data-based reconstructions provide constraints in terms of the field morphology at the Earth’s surface and at the core-mantle boundary. Such models are constrained by direct measurements for recent periods and by indirect data for older intervals. For the time span covering the last few centuries to approximately 50 ka, the available paleomagnetic data are unevenly distributed in both space and time, with a strong bias toward the Northern Hemisphere and more recent periods. These data limitations influence the reliability of geomagnetic model predictions, particularly in poorly sampled regions such as South America. In recent years, new paleomagnetic data have been obtained from ocean-floor sediments off the southern coast of Brazil. However, integrating paleomagnetic data from geographically close locations, together with reliable age and sedimentation rate models, remains a major challenge and limits the reproducibility of records from nearby sites. To address this issue, we applied a machine-learning approach based on Gaussian process regression to construct inclination and relative paleointensity curves using data from three sediment cores collected in this region (29°S, 47°W). This method allows for the estimation of a modeled curve that integrates data from the three cores, which have irregular time intervals between samples, and provides associated uncertainties. The resulting inclination and relative paleointensity curves were compared with predictions from the GGF100k geomagnetic model. Overall, the results show good agreement with model predictions, although some discrepancies are observed in both inclination and intensity over the studied interval. These findings demonstrate that Gaussian process regression is a robust and effective tool for integrating paleomagnetic data from oceanic sediment cores.

How to cite: Frigo, E., Gomes Gonçalves, Í., Francisco Savian, J., Yesid Suárez-Ibarra, J., Panovska, S., André Hartmann, G., Azzolini Pontel, C., Trindade Lopes, C., Alejandra Gómez Pivel, M., Carlos Coimbra, J., Monticelli Petró, S., Leonhardt, A., and Ivan Ferreira da Trindade, R.: Paleomagnetic variations along the Southern Coast of Brazil from 46.06-5.36 ka BP using a Gaussian Process Technique, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11365, https://doi.org/10.5194/egusphere-egu26-11365, 2026.

EGU26-11382 | Posters on site | EMRP3.3

Astronomical tuning of the Late Cretaceous geomagnetic polarity time scale (from top Chron C34n to base Chron C30n) 

Edoardo Dallanave, Thomas Westerhold, and Alexandra Villa

The Geomagnetic Polarity Time Scale (GPTS) is the backbone of the time scale for at least the last ~84 Myr (Late Cretaceous–Quaternary). Astronomically calibrated ages for the Cenozoic portion (C-Sequence) of the GPTS are provided as part of the Cenozoic Global Reference benthic foraminifer carbon and oxygen Isotope Dataset (CENOGRID1), but not for the late Cretaceous portion of the C-Sequence. We aim to provide astronomically calibrated age for the late Cretaceous magnetic Chron boundaries. We generated preliminary magnetic polarity stratigraphy data and bulk carbon stable isotope data from a series of deep-sea drilled record recovered in the South Atlantic Ocean: Ocean Drilling Program (ODP) Site 1267 2 (Leg 208), Deep Sea Drilling Project (DSDP) Site 5253 (Leg 74), and International Ocean Drilling Project (IODP) Site U15764 (Exp. 391) from Walvis Ridge, and DSDP Site 5165 (Leg 72) from the Rio Grande rise. The sampled records are generally characterized by a stable magnetic remanence with either normal (up-pointing) or reverse (down-pointing) inclination of the remanence vector. The integration of magneto- and carbon isotope-stratigraphy will be used to calibrate the GPTS from the top of Chron C34n to the base of Chron C30n. To achieve this, we will use a new approach based on the correlation of the obtained magnetostratigraphy to an astronomically tuned reference by using the bulk carbonate stable carbon isotope data. This effort represents the first step toward a fully astronomically calibrated C-sequence of the GPTS that is consistent with CENOGRID.

 

References

1 Westerhold, T. et al. An astronomically dated record of Earth’s climate and its predictability over the last 66 million years. Science (1979) 369, 1383–1388 (2020).

2 Zachos, J. C., Kroon, D. & Blum, P. Site 1267. Proceedings of the Ocean Drilling Program, 208 Initial Reports 208, 1–77 (2004).

3 Chave, A. D. Lower Paleocene–Upper Cretaceous magnetostratigraphy, Sites 525,527, and 529, Deep Sea Drilling Project Leg 74. in Deep Sea Drilling Project preliminary report, Vol. 74 (eds. Moore, T. C. & Rabinowitz, P. D.) 525–531 (DSDP, Washington DC, USA, 1984). doi:10.2973/dsdp.proc.74.1984.

4 Sager, W. et al. Site U1576. International Ocean Discovery Program: Preliminary Reports 391, 1–65 (2023).

5 Barker, P. F., Carlson, R. L., Johnson, D. A. & Al., E. Site 516. Deep Sea Drilling Project preliminary report, Vol. 72 (1983).

How to cite: Dallanave, E., Westerhold, T., and Villa, A.: Astronomical tuning of the Late Cretaceous geomagnetic polarity time scale (from top Chron C34n to base Chron C30n), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11382, https://doi.org/10.5194/egusphere-egu26-11382, 2026.

EGU26-11479 | Orals | EMRP3.3

Paleomagnetic records of Matuyama chron and beyond from North Atlantic drift sediments: IODP Expedition 384/395C/395 sites 

Anita Di Chiara, Sara Satolli, Sarah Friedman, Deepa Dwyer, Gary Acton, Boris Theofanis Karatsolis, Tom Dunkley Jones, Paul N. Pearson, Takuma Suzuki, Anne Briais, Ross Parnell-Turner, Leah LeVay, and Expedition 395 Science Party

Drift sediments in the North Atlantic accumulated rapidly (≥10 cm/kyr) over the past ~3.6 Ma, enabling high-resolution reconstructions of geomagnetic field behavior. Previous scientific drilling expeditions (e.g., ODP Leg 162, IODP Exp. 306) from the North Atlantic refined the Quaternary Geomagnetic Instability Time Scale (GITS; 0–2.58 Ma) by revealing short-lived geomagnetic instabilities like the Iceland Basin Excursion (~188 ka). Here, we aim at further refining the GITS by studying newly collected cores in the same area.

Between 2020 and 2023, the International Ocean Discovery Program (IODP) Expeditions 384, 395C, and 395 targeted six sites: five along a transect east of the Mid-Atlantic Ridge (20–30°W, ~60°N) and one west of Greenland. These expeditions targeted the volcanic basement that forms the V-shaped ridges/troughs on the Reykjanes Ridge and the overlying sediments that record deepwater current evolution. Shipboard age models are based on paleomagnetic and microfossil data, but a robust and reliable paleomagnetic record extends up to 11 Ma.

We present results from Expeditions 384/395C/395 sediments that capture most GITS magnetic events (excursions and reversals) within the Matuyama chron. These records hold potential to extend the GITS backward in time, bolstering magnetic instabilities as geochronologic tools and refining models of Earth's ancient geomagnetic variations.

How to cite: Di Chiara, A., Satolli, S., Friedman, S., Dwyer, D., Acton, G., Karatsolis, B. T., Dunkley Jones, T., Pearson, P. N., Suzuki, T., Briais, A., Parnell-Turner, R., LeVay, L., and 395 Science Party, E.: Paleomagnetic records of Matuyama chron and beyond from North Atlantic drift sediments: IODP Expedition 384/395C/395 sites, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11479, https://doi.org/10.5194/egusphere-egu26-11479, 2026.

EGU26-11884 | ECS | Orals | EMRP3.3

LAVA: A machine learning method for predicting absolute paleointensities from pseudo-Thellier data  

Liz van Grinsven, Djurre van der Molen, Bertwin M. de Groot, Sara Langelaar, and Lennart V. de Groot

Reliable paleointensity estimates are crucial for understanding past behavior of the Earth’s magnetic field but remain difficult to obtain using traditional methods. Conventional thermal Thellier paleointensity experiments often have low success rates for volcanic samples, as repeated heating can induce alteration. Heating can be avoided by using the pseudo-Thellier method, in which samples are magnetized using alternating fields. However, pseudo-Thellier experiments intrinsically yield only relative paleointensities.

Over the past years, several attempts have been made to calibrate pseudo-Thellier results to absolute paleointensities for lavas by relating laboratory-induced anhysteretic remanent magnetizations (ARMs) to the thermally acquired natural remanent magnetizations (NRMs). Because magnetization depends on factors such as magnetic grain size, shape, and minerology, simple linear models struggle to consistently predict paleointensities across varied datasets.

Here, we present LAVA (Learning Absolute paleointensities from Volcanic ARMs), a machine learning approach that predicts absolute paleointensities from pseudo-Thellier data. Machine learning methods are well suited to model highly non-linear and complex relationships between ARM and NRM. LAVA was calibrated and tested using two datasets: a synthetic laboratory-induced datasets and a dataset of recently cooled volcanic products from diverse volcanic settings and geographic locations whose natural remanent magnetizations span the full range of observed geomagnetic field strengths. LAVA outperforms existing pseudo-Thellier interpretation techniques, by predicting the paleointensity for every volcanic site in the natural dataset within 5.6 μT and with an average error of 1.3 μT. These results demonstrate that LAVA provides a robust new tool for recovering absolute paleointensities from volcanic rocks.

How to cite: van Grinsven, L., van der Molen, D., de Groot, B. M., Langelaar, S., and de Groot, L. V.: LAVA: A machine learning method for predicting absolute paleointensities from pseudo-Thellier data , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11884, https://doi.org/10.5194/egusphere-egu26-11884, 2026.

EGU26-12741 | ECS | Posters on site | EMRP3.3

Time dependence of multiple geomagnetic surface intensity minima 

Yaochen Yue, Hagay Amit, Filipe Terra-Nova, Victor Marum, Yuqi Wang, and Yong Wei

The present-day geomagnetic field is characterized by a region of weak intensity over the South Atlantic, known as the South Atlantic Anomaly (SAA). Over the past few hundred years, there is evidence for possible persistence of the SAA. In addition, another less pronounced surface intensity minimum has appeared below the West Pacific, known as the West Pacific Anomaly (WPA). Since 2008, the SAA has split with a new local minimum appearing in Africa. This split introduces a challenge for characterizing the time dependence of a pair of minima, particularly in terms of their respective areas.

In this work, we propose a new topological algorithm to calculate the time dependent areas and centers of complex field configurations with multiple local surface intensity minima enclosed by the same threshold value. The algorithm relies on the identification of saddle points, which further enables the subdivision of the SAA area into sub-regions associated with different minima. In addition, the analysis considers contours of null intensity gradient, which do not require setting an arbitrary threshold value.

Based on the analysis of a modern geomagnetic field model, we find that the sub-region area associated with the weaker South American minimum decreases, whereas that of the African minimum increases. Both minima drift westward with negligible north-south displacement. The global minimum is located at a lower latitude than both local minima. The proposed method can be applied to paleo-magnetic field models, in which more complex patterns are observed.

In addition, analysis of the distribution of the null meridional intensity gradient over the period 1000–1950 reveals localized hemispheric asymmetry with relatively subdued activity in the Pacific hemisphere and stronger variability in the Atlantic, particularly in the Southern Hemisphere. The null intensity azimuthal gradient exhibits an order-2 signature suggestive of mantle control on the geomagnetic field.

How to cite: Yue, Y., Amit, H., Terra-Nova, F., Marum, V., Wang, Y., and Wei, Y.: Time dependence of multiple geomagnetic surface intensity minima, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12741, https://doi.org/10.5194/egusphere-egu26-12741, 2026.

EGU26-12826 | Orals | EMRP3.3

Identifying chemical remanent magnetization in marine sediments via anhysteretic magnetization: Case study from the Bermuda Rise, North Atlantic Ocean   

Stuart Gilder, Michael Wack, Sophie Roud, Felix Ostermeier, Josef Jezek, and David Finn

Paleomagnetic studies of marine sediments often assume that the remanence acquisition process occurs via torque from the Earth's magnetic field called a depositional remanent magnetization (DRM), which implies that paleomagnetic recording is time-transgressive. However, magnetic minerals can also grow authigenically in the sediment, leading to a chemical remanent magnetization (CRM), which is not necessarily time-transgressive. Not only are the physics of the DRM and CRM acquisition processes different, but their remanence lock-in times are likely non-contemporaneous, potentially leading to misinterpretations of the magnetic signal. The question arises how to distinguish the two? The hallmark of a detrital remanence can be expressed by the anisotropy of remanence. Since single domain prolate grains should be distributed statistically parallel to the magnetic field direction, the maximum anisotropy axis should also be in the magnetic field direction, as suggested by our theoretical models and confirmed by our experimental data. But what about CRM? To test this, we applied a wide range of experiments using anhysteretic methods with the automated SushiBar system on Bruhnes-Matuyama-aged marine sediments from the Bermuda Rise (ODP Site 1063). Previous work assumed the remanence in these sediments was carried solely by magnetite; however, we found evidence for a gyroremanent magnetization (GRM), which is commonly attributed to greigite. Of interest is that these samples, as well as neighboring samples or other intervals that do not show evidence for GRM, yield distinctly different characteristics either in their remanence anisotropy parameters and/or in their partial anisotropy spectra. We present new methodology that helps identify potential CRM-bearing horizons that was overlooked by existing techniques.

How to cite: Gilder, S., Wack, M., Roud, S., Ostermeier, F., Jezek, J., and Finn, D.: Identifying chemical remanent magnetization in marine sediments via anhysteretic magnetization: Case study from the Bermuda Rise, North Atlantic Ocean  , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12826, https://doi.org/10.5194/egusphere-egu26-12826, 2026.

EGU26-13078 | ECS | Orals | EMRP3.3

Testing the Geomagnetic Axial Dipole hypothesis at the South Atlantic Anomaly region 

Victor Marum, Gelvam Hartmann, Filipe Terra-Nova, Hagay Amit, Yaochen Yue, Marina Puente-Borque, and Ricardo Trindade

A robust reconstruction of geomagnetic field intensity requires careful evaluation of spatial sampling strategies and latitude reduction methods, especially in regions strongly influenced by non-dipolar field components. In this work, we systematically investigate the statistical stability and spatial and temporal sensitivity of regional geomagnetic intensity estimates as a function of three fundamental variables: the radius of the spatial region used to represent a point of interest, the number of sites sampled within the region of interest and the number of independent site samples. Using the global geomagnetic field models CHAOS-8.1 and COV-OBS.x2, we simulated controlled statistical experiments in which field intensity values ​​are randomly sampled in circular regions centered on previously defined locations of interest. Five locations were analyzed, including two fixed points (Paris and São Paulo cities) and three time-varying reference points associated with the minimum, maximum and average values ​​of the paleosecular variation index (Pi). The statistical performance of the regional estimates was quantified using the normalized root-mean-square (RMS) error, calculated relative to the local reference intensity at a specific epoch. Five approaches were tested: (i) without latitude correction; (ii) latitude correction considering only the axial dipole term (g10); (iii) latitude correction including the axial dipole and quadrupole terms (g10 + g20); (iv) latitude correction including axial dipole, quadrupole and octupole terms (g10 + g20 + g30); and (v) the eccentric dipole (ED) approximation. Our results show that the sampling radius is the dominant parameter in controlling the error. The effectiveness of the latitude corrections strongly depends on the region and epoch analyzed. Axial latitude corrections perform better in contexts close to a dipolar configuration, while no latitude correction or ED approach are more effective in regions dominated by non-dipolar contributions, such as the South Atlantic Anomaly (SAA).

How to cite: Marum, V., Hartmann, G., Terra-Nova, F., Amit, H., Yue, Y., Puente-Borque, M., and Trindade, R.: Testing the Geomagnetic Axial Dipole hypothesis at the South Atlantic Anomaly region, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13078, https://doi.org/10.5194/egusphere-egu26-13078, 2026.

EGU26-15640 | ECS | Posters on site | EMRP3.3

Preliminary Paleomagnetic and Rock Magnetic Results from the Aptian–Albian Marne a Fucoidi Formation at Monte Cucco (Hill 991), Italy 

Raquel Gewehr de Mello, Jairo Francisco Savian, Carolina Gonçalves Leandro, Fabrizio Frontalini, Anita Di Chiara, Caroline Azzolini Pontel, Rodolfo Coccioni, and Nicola Casadei

The Aptian-Albian interval represents a key phase in Earth history, characterized by greenhouse climate conditions, major perturbations in oceanic redox state and significant changes in geomagnetic field behavior leading to the establishment of the Cretaceous Normal Superchron (CNS). Here we present an ongoing paleomagnetic and rock magnetic study of the Monte Cucco (“Hill 991”) section, located on the western margin of the Umbria–Marche Apennines. The section belongs to the Umbria–Marche Succession and preserves a continuous upper Aptian–lower Albian stratigraphy record within the Marne a Fucoidi Formation, a cyclic marly–calcareous characterized by alternating marls, clay-rich marls, and calcareous levels, including organic-rich horizons and black shales associated with Oceanic Anoxic Events (OAE), particularly OAE1b. The dataset includes stepwise alternating field and thermal demagnetization to isolate the characteristic remanent magnetization, complemented by rock magnetic analyses such as magnetic susceptibility, anhysteretic remanent magnetization (ARM), isothermal remanent magnetization (IRM), and coercivity component analysis. These analyses are currently in progress and will be completed to constrain magnetic mineralogy, grain-size distribution, and environmental controls on the magnetic signal across lithological cycles and OAE-related intervals. Preliminary paleomagnetic results indicate stable characteristic remanent magnetization components. Hysteresis parameters and IRM acquisition curves suggest a mixed magnetic assemblage dominated by low-coercivity magnetite, with grain sizes ranging from single-domain (SD) to pseudo-single-domain (PSD) and a subordinate contribution of multi-domain (MD) grains. The assemblage is predominantly detrital, with local variations suggesting a relative enrichment in finely grained magnetite. The final dataset will be integrated with existing Poggio le Guaine (PLG), a Aptian-Albian complete record located approximately 20 km from Monte Cucco and compared with magnetostratigraphic data from South Atlantic marginal basins, particularly the Brazilian Equatorial Margin. This approach aims to strengthen interbasinal correlations between the Tethyan realm and Gondwanan margins and to refine constraints on geomagnetic field behavior and paleoenvironmental variability during the Aptian–Albian transition.

How to cite: Gewehr de Mello, R., Francisco Savian, J., Gonçalves Leandro, C., Frontalini, F., Di Chiara, A., Azzolini Pontel, C., Coccioni, R., and Casadei, N.: Preliminary Paleomagnetic and Rock Magnetic Results from the Aptian–Albian Marne a Fucoidi Formation at Monte Cucco (Hill 991), Italy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15640, https://doi.org/10.5194/egusphere-egu26-15640, 2026.

EGU26-15642 | ECS | Posters on site | EMRP3.3

Building upon the paleomagnetic history of mafic intrusions in the pre-North American Mid-Continent Rift system, Western Upper Peninsula of Michigan. 

Gabriel Ahrendt, Miah Mol, Leonid Surovitskii, and Aleksey Smirnov

The Western Upper Peninsula of Michigan (WUP), located in the north-central United States, is part of the Paleoproterozoic North American Continent accreted onto the ~2.6 Ga Superior craton. The WUP is intersected by several generations of diabase dikes associated with the ~1.1 Ga North American Mid-Continent Rift system (MCR). In addition to these dikes, recent aeromagnetic and geological surveys of the WUP have revealed multiple sets of dikes in the southeastern and north-northeastern portions of the region that trend either perpendicular or obliquely to the MCR rift axis. Geological relationships derived from stratigraphic field studies, along with paleomagnetic and geochemical analyses, suggest that these dikes predate the Keweenawan dikes of the main-stage MCR, likely dating to the early Mesoproterozoic to late Paleoproterozoic. The dikes in the southeastern part of the WUP intrude the Archean Carney Lake Gneiss Complex (CLGC) and can be subdivided into several small but distinct swarms with varying orientation and geomagnetic polarities. These findings point to a possible circumferential dike structure (Buchan and Ernst, 2019)1 of middle Paleoproterozoic age at the locus of the CLGC. A set of dikes located directly North of the CLGC, in the Neoarchean Dickinson Group, were also sampled to test this theory and constrain the region’s metamorphic conditions. Meanwhile, newly obtained geochemical data from dikes belonging to three distinct swarms in the north-central to northeastern portion of the region provide support for previous paleomagnetic interpretations linking these swarms to the earliest stages of hotspot activity which indicate the onset of the MCR. Further, new paleomagnetic and geochemical data collected from north-south trending dikes of the Huron Mountains in the northernmost portion of the northeast WUP, were analyzed to determine if they are constituent to the ~2.1 Ga Marathon dike swarm in Ontario, Canada, or evidence of fault-fracture infilling caused by the onset of the main stage MCR volcanism. We will present new results of geochemical, paleomagnetic, and rock-magnetic investigations of the pre-MCR dikes in the WUP and discuss their implications to the regional tectonic history.

[1] Buchan, K.L., Ernst, R.E. (2019). Giant Circumferential Dyke Swarms: Catalogue and Characteristics. In: Srivastava, R., Ernst, R., Peng, P. (eds) Dyke Swarms of the World: A Modern Perspective. Springer Geology. Springer, Singapore. https://doi.org/10.1007/978-981-13-1666-1_1

How to cite: Ahrendt, G., Mol, M., Surovitskii, L., and Smirnov, A.: Building upon the paleomagnetic history of mafic intrusions in the pre-North American Mid-Continent Rift system, Western Upper Peninsula of Michigan., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15642, https://doi.org/10.5194/egusphere-egu26-15642, 2026.

EGU26-15660 | Orals | EMRP3.3

Revisiting the Mono Lake Excursion Type Section with High-Resolution Paleomagnetic Records 

Britta Jensen, Daniel Ibarra, Alberto Reyes, Serhiy Buryak, Michael Evans, and Vadim Kravchinsky

The Wilson Creek Formation, exposed around Mono Lake in east-central California, is comprised of interbedded lacustrine sediments and tephra that were deposited during higher stands of Mono Lake (Lake Russell) in the late Pleistocene. A prominent paleomagnetic excursion recorded in this formation led to the recognition and naming of the ~33 ka Mono Lake geomagnetic excursion (MLE). However, recent direct radiometric dating of key tephra layers bracketing this event have shown that this excursion is instead the Laschamps geomagnetic excursion (~41 ka). This has prompted a recommendation (e.g., Laj et al., 2014) that the MLE be renamed the "Auckland excursion," based on a reliably dated and well-documented paleomagnetic record for a ~33 ka excursion in New Zealand, casting doubt on the presence of the MLE at its namesake site.

Nevertheless, close inspection of paleomagnetic profiles from two pioneering studies suggest that there may be a second, less prominent, paleomagnetic anomaly above the Laschamps. The striking lateral continuity of the Wilson Creek Formation and its prominent tephra layers facilitates the identification and resampling of the intervals of interest. We carried out high-resolution paleomagnetic sampling of three trenches bracketed by key dated tephra, focussing on the interval between Ash 8 (~34 ka) and Ash 7 (~26 ka), the location of the potential second anomaly, with one trench extending below Ash 15 (~42 ka) to capture the Laschamps excursion. Thermal demagnetization revealed that the lacustrine sediments of Mono Lake are excellent paleomagnetic recorders, with well-behaved remanence directions. Below Ash 15, the sediments contain a sharp and well-defined excursion consistent with the Laschamps excursion. Most significantly, all the trenches reveal a coherent pattern of significantly reduced inclinations between Ashes 8 and 7, with values dipping below 20° without full polarity reversal. This pattern, present in all three trenches, is defined by a double-dip inclination structure and westward-shifting declinations. These findings show that while the original excursion identified at Mono Lake is instead the Laschamps excursion, the MLE is indeed recorded at Mono Lake with an age of ~33 ka consistent with current estimates. Moreover, the enhanced resolution afforded by high sedimentation rates may be capturing previously underappreciated complexity in the geomagnetic field behavior during this excursion.

How to cite: Jensen, B., Ibarra, D., Reyes, A., Buryak, S., Evans, M., and Kravchinsky, V.: Revisiting the Mono Lake Excursion Type Section with High-Resolution Paleomagnetic Records, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15660, https://doi.org/10.5194/egusphere-egu26-15660, 2026.

EGU26-15717 | Posters on site | EMRP3.3

Paleomagnetic preliminary results from the Aptian-Albian Araripe Basin, northeastern Brazil 

Jairo Savian, João Ramos, Caroline Pontel, Josefa Lacerda, Juliano Kuchle, Roberto Silva Jr, Raquel de Mello, Camila Lopes, Sofia Nunes, Gabrieli Almeida, and Milene Figueiredo

Tectonic opening of the Equatorial Atlantic Gateway (EAG) and its impact on Ocean–Atmosphere dynamics has global implications. Rifting between South America and Africa drove a transition from continental–lacustrine to evaporitic, and ultimately marine, environments, although the timing and duration of these changes remain debated. Over the same period, Earth’s magnetic field remained in a stable polarity state for ~38 Myr, a phase referred to as the Cretaceous Normal Superchron (CNS). In northeastern Brazil we have key sedimentary sections for this period, such as the Araripe Basin. The studied interval within the basin is notable for recording the evolution from restricted marine sequences to the complete opening of the EAG. Here, we present a preliminary paleomagnetic study of key sedimentary sections from Araripe Basin, in northeastern Brazil, covering the Aptian-Albian ages. Stepwise alternating field (AF) and thermal (TH) demagnetizations were used to isolate the primary remanent component. Magnetic remanence and rock magnetic parameters, such as magnetic susceptibility (χ), anhysteretic remanent magnetization (ARM) and isothermal remanent magnetization (IRM), were measured. Rock magnetic measurements indicate that the primary magnetic remanence carriers are low-coercivity magnetite and/or titanomagnetite and high-coercivity hematite. Our magnetoestratigraphy records reveal a long interval of normal polarities associated with the CNS, with isolated short intervals of reversed polarities that could be further investigated in the future. The results illustrate the potential of paleomagnetic records for best understanding the Earth’s magnetic field in the equatorial region during the Aptian-Albian to better understanding the age and tectonic evolution of the EAG.

How to cite: Savian, J., Ramos, J., Pontel, C., Lacerda, J., Kuchle, J., Silva Jr, R., de Mello, R., Lopes, C., Nunes, S., Almeida, G., and Figueiredo, M.: Paleomagnetic preliminary results from the Aptian-Albian Araripe Basin, northeastern Brazil, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15717, https://doi.org/10.5194/egusphere-egu26-15717, 2026.

EGU26-17232 | Orals | EMRP3.3

Full-vector Holocene records from Réunion and Bali constrain the origin of the South Atlantic Anomaly 

Lennart de Groot, Romy Meyer, Aditya Pratama, Ahmad Fadillah, and Liz van Grinsven

The South Atlantic Anomaly (SAA) is the most prominent low-intensity feature of the modern geomagnetic field. Its origin is debated between hypotheses invoking (i) a deep-mantle controlled flux system beneath southern Africa at the edge of the African Large Low-Shear Velocity Province (LLSVP), and (ii) models proposing an eastward origin in the Indian Ocean followed by westward migration into the South Atlantic. Discriminating between these scenarios requires well-dated Southern Hemisphere paleomagnetic records, which remain sparse.

Here, we present new full-vector paleomagnetic data from volcanic products on Réunion Island and Bali (Indonesia), providing constraints on Holocene field behavior on both sides of the Indian Ocean. At Réunion, Bayesian paleosecular-variation curves based on our new data reveal a pronounced intensity maximum around ~1400 CE followed by a sharp decline to ~29 µT at ~1550 CE. This high-to-low transition indicates that Réunion did not experience persistent low fields prior to the devolpment of the SAA. This is inconsistent with models proposing an origin under the Indian Ocean and an east-to-west migration from there. Instead, the Réunion record documents the onset of low-field behavior only after ~1400 CE, in agreement with the hypothesis that the SAA originated below, or slightly to the east of the African continent and is probably linked to the presence of the African LLSVP.

The Indonesian paleointensity records from Bali reveal earlier low-intensity episodes (~1000–1300 CE), but these are temporally disconnected from the Réunion minimum and are best interpreted as expressions of independent or recurrent (West) Pacific or Indian Ocean anomalies rather than precursors of the SAA. Together, the data indicate that while low-field patches may likely  recur in the Indian Ocean realm, the modern SAA originated beneath southern Africa and moved westwards from its point of inception. These results support a top-down control on the geodynamo driving the occurence of the SAA and provide new data to create the next-generation geomagnetic field models optimized to track the origin, and. evolution of the South Atlantic Anomaly through time.

How to cite: de Groot, L., Meyer, R., Pratama, A., Fadillah, A., and van Grinsven, L.: Full-vector Holocene records from Réunion and Bali constrain the origin of the South Atlantic Anomaly, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17232, https://doi.org/10.5194/egusphere-egu26-17232, 2026.

EGU26-17477 | ECS | Orals | EMRP3.3

Latitude-dependent sensitivity of 10Be records to variations in geomagnetic field intensity 

Julia Loftfield, Vincent Wall, Minjie Zheng, Konstanze Stübner, Johannes Lachner, Georg Rugel, and Florian Adolphi

The atmospheric production rate of cosmogenic 10Be is inversely related to the geomagnetic field strength. This leads to variable deposition rates of 10Be in environmental archives, such as ice or sediment cores. 10Be records from these archives can, therefore, be used to reconstruct past intensities of the geomagnetic field. Recent 10Be production and atmospheric mixing models, however, suggest that the sensitivity of 10Be records to changes in the geomagnetic field intensity depends on the latitude. This impacts the use of single-site 10Be records for reconstructing global 10Be production rates and, therefore, geomagnetic field intensities.

Here, we quantitatively assess the latitudinal sensitivity of 10Be deposition to geomagnetic field changes. We present new authigenic 10Be/9Be data from a sediment core from the Bay of Bengal (IODP U1446) and compile additional 10Be data from ice and sediment cores. Our analysis focuses on 10Be deposition changes during the Laschamps geomagnetic field intensity minimum at different latitudes. We compare 10Be deposition changes with changes in modeled 10Be production from geomagnetic field reconstructions (LSMOD.2, GGFSS70, Black Sea, GLOPIS-75) and the GEOS-Chem atmospheric mixing model.

Our findings reveal that 10Be deposition changes are larger in the tropics (tropical enhancement) and diminish at higher latitudes (polar bias), indicating incomplete mixing of cosmogenic beryllium, consistent with atmospheric mixing models. This latitudinal sensitivity needs to be taken into account when reconstructing variations in global geomagnetic field intensity from 10Be. 

How to cite: Loftfield, J., Wall, V., Zheng, M., Stübner, K., Lachner, J., Rugel, G., and Adolphi, F.: Latitude-dependent sensitivity of 10Be records to variations in geomagnetic field intensity, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17477, https://doi.org/10.5194/egusphere-egu26-17477, 2026.

EGU26-18433 | Orals | EMRP3.3

A promising novel recorder of Earth’s ancient magnetic field: fossil micrometeorites as paleomagnetic archives 

Annique van der Boon, Rosa de Boer, Bertwin de Groot, Hans Arne Nakrem, Lisa Krämer Ruggiu, Steven Goderis, and Lennart de Groot

The paleomagnetic record from sedimentary rocks is often ambiguous, limiting the recovery of reliable paleomagnetic data, particularly when compared to paleomagnetic data obtained from igneous rocks. We explore the potential of a novel type of paleomagnetic recorder in sedimentary rocks: fossil micrometeorites. Micrometeorites (MM) are small cosmic particles (50 μm-2mm) which account for a significant portion of the approximately 40,000 tons of extraterrestrial material that arrives on Earth annually. Many MMs melt during atmospheric entry, at altitudes of 80-90 km and transform into cosmic spherules (CS). CS have long been recognised as magnetic and can be extracted from sedimentary rocks. During melting and formation of CS, MM oxidise and form new minerals, particularly wüstite and magnetite. Subsequently, the cosmic spherules quench within a few seconds. This rapid cooling through the Curie temperature leads to the formation of thermoremanent magnetisations within CS. Diagnostic features such as metal beads and vesicles inside a proportion of CS make it possible to determine their flight trajectory, which can be combined with the magnetisation to reconstruct the polarity of EMF. While modern CS from Antarctica have already been shown to be good recorders of the geomagnetic field1, the deep-time paleomagnetic records of CS remain unexplored. We present the results of a paleomagnetic study of anthropogenic magnetite spherules that resemble iron-type (I-type) CS, as well as several Paleozoic I-type CS. We demonstrate that individual spherules are measurable using existing paleomagnetic methods and equipment, while computed tomography (NanoCT) scanning enabled reliable reconstruction of the fall trajectory of a Paleozoic CS. We show that fossil CS with sizes of 50-300 μm are a promising, novel class of paleomagnetic recorder, accessible with existing techniques and capable of opening a new window on the ancient geomagnetic field.

1Suavet, C., Gattacceca, J., Rochette, P. & Folco, L. Constraining the terrestrial age of micrometeorites using their record of the Earth’s magnetic field polarity. Geology 39, 123–126 (2011).

How to cite: van der Boon, A., de Boer, R., de Groot, B., Nakrem, H. A., Krämer Ruggiu, L., Goderis, S., and de Groot, L.: A promising novel recorder of Earth’s ancient magnetic field: fossil micrometeorites as paleomagnetic archives, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18433, https://doi.org/10.5194/egusphere-egu26-18433, 2026.

EGU26-20144 | ECS | Posters on site | EMRP3.3

Tracking the ETM3, ETM2, and PETM hyperthermal events: New Age Model and Magnetostratigraphic Study  

Raquel Bonilla-Alba, Anita Di Chiara, Fabio Florindo, and Paola De Michelis

This work studies focuses on periods of dramatic temperature changes during the early Eocene hyperthermal events ETM3 (~52.8 Ma), ETM2 (~54 Ma), and the PETM (~56 Ma). We aim at developing a refined age model for IODP Site U1514 (Mentelle Basin) and carry out a suite of rock magnetic measurements as proxies for paleoclimatic changes. On 234 sediment samples from 248.2 to 324.68 m CSF-A we performed new magnetic measurements including AF demagnetization, AMS (Anisotropy of Magnetic Susceptiblity), bulk susceptibility, IRM (Isothermal Remanent Magnetization) acquisition and demagnetization, and ARM (Anysteretic Remanent Magnetization) acquisition and demagnetization. The integration of these new data with the previously available shipboard datasets allows us to characterise magnetic mineral assemblages, remanence carriers, and sedimentary processes at a resolution not previously available for this site. The new high-resolution paleomagnetic (Inclination only) data allow a clearer identification of polarity boundaries and reduce uncertainties in the placement of chron transitions. This improved temporal control enables a more precise determination of the depths and thicknesses of ETM3, ETM2, and the PETM. Variations in ARM/k ratios, IRM acquisition curves, and susceptibility reveal changes in magnetic grain size and concentration that align with intervals of elevated temperature. Applying Fourier transforms to continuous magnetic property curves, constructed from magnetic parameters, allowed us to detect statistically significant cyclicity consistent with short and long eccentricity. These Milankovic oscillations provide independent constraints on sedimentation rates and help refine accumulation histories surrounding the hyperthermal intervals. The orbital pacing observed in the background sedimentation also strengthens the reliability of the new age model. By combining the refined magnetostratigraphy, magnetic property analyses, and orbital cyclicity, we produce a high-quality framework to identify and correlate ETM3, ETM2, and the PETM. This improved temporal and stratigraphic resolution clarifies the relative timing between warming, environmental shifts, and changes in sediment properties.

How to cite: Bonilla-Alba, R., Di Chiara, A., Florindo, F., and De Michelis, P.: Tracking the ETM3, ETM2, and PETM hyperthermal events: New Age Model and Magnetostratigraphic Study , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20144, https://doi.org/10.5194/egusphere-egu26-20144, 2026.

EGU26-21857 | Orals | EMRP3.3

Interpretation of palaeomagnetic signals from palaeo-lake sediments of the Atacama (Chile) – evidence of geomagnetic excursions in C5Cn.1n? 

Stephanie Scheidt, Volker Wennrich, Richard Albert, Niklas Leicher, Ascelina Hasberg, Scott D. McLin, Julia J. Diederich-Leicher, Christian Zeeden, and Martin Melles

Sediment cores recovered from the Playa Adamito Grande (PAG) claypan in the hyperarid core of the Atacama Desert (Chile) show a sequence of three main lithological units. Here we focus on the lowest unit, which was found below 29.2 m to the bottom of the core at a depth of 52 m. The silty-clayey sediment is frequently interspersed with gypsum-rich layers and is interpreted as a palaeo-lake deposit. At the top of this unit an erosion unconformity was identified at ca. 29.5 m depth. Two U/Pb zircon ages obtained from tephra layers provide chronological data at 31.49 m (16.27 ± 0.09 Ma) and 29.22 m (15.54 ± 0.03 Ma) sediment depth.  Below, none of the various dating methods employed yielded results. The timing and duration of the lake phase in the Atacama, were therefore attempted to be determined more precisely using magnetic polarity stratigraphy. The mineral magnetic association is composed of partially maghemised magnetite and Ti-magnetite in domain states that allow for retention of the magnetic signal over long geological time scales. However, the sediment sequence mainly exhibits normal polarity, interrupted only by thin layers with reversed polarity. Therefore, it is not readily possible to specify age constraints for the lake phase by correlation with the geomagnetic polarity time scale (GPTS). Some of the layers with reversed polarity coincide with layers rich in gypsum. Therefore, we discuss the nature of these short-lived reversed sections, considering possible post-depositional overprinting of the magnetic signal or the occurrence of hiatuses. However, our considerations show that the palaeomagnetic signal most likely represents a high-resolution record of field instabilities during the Miocene. This interesting case study thus provides new evidence for the occurrence of geomagnetic excursions during the Subchron C5Cn.1n (Middle Miocene).

How to cite: Scheidt, S., Wennrich, V., Albert, R., Leicher, N., Hasberg, A., McLin, S. D., Diederich-Leicher, J. J., Zeeden, C., and Melles, M.: Interpretation of palaeomagnetic signals from palaeo-lake sediments of the Atacama (Chile) – evidence of geomagnetic excursions in C5Cn.1n?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21857, https://doi.org/10.5194/egusphere-egu26-21857, 2026.

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