EGU26-19008, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-19008
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Thursday, 07 May, 16:15–18:00 (CEST), Display time Thursday, 07 May, 14:00–18:00
 
Hall X1, X1.104
Imaging of Serpentinites beneath the Münchberg Massif (Germany) using Joint Gravity and Magnetic Inversion
Peter Klitzke1, Mohamed Sobh2, Antonia Ruppel1, Meike Bagge1, Nikola Koglin1, Maximilian Hasch1, Rodolfo Christiansen2, Hamed Fazlikhani3, Jan-Felix Goldmann1, Ingo Heyde1, and Alexander Löwer4
Peter Klitzke et al.
  • 1Federal Institute for Geosciences and Natural Resources (BGR), Energy Resources and Polar Geology, Hannover, Germany (peter.klitzke@bgr.de)
  • 2Leibniz Institute for Applied Geophysics (LIAG), Hannover, Germany
  • 3GeoZentrum Nordbayern, Friedrich-Alexander-Universität (FAU) Erlangen-Nürnberg, Germany
  • 4iMAR Navigation GmbH, St. Ingbert, Germany

Serpentinisation is a water–rock reaction in ultramafic lithologies that can generate natural hydrogen and strongly modifies rock density and magnetic susceptibility. Quantifying the spatial distribution of serpentinized bodies is therefore essential for assessing the subsurface potential of natural hydrogen systems.

The Münchberg Massif (northern Bavaria, Germany) is an exhumed stack of tectonic nappes of different metamorphic grades that hosts several outcropping serpentinite bodies. This provides a rare opportunity to study serpentinisation in a setting that is typically buried at considerable crustal depths. The serpentinites are mainly exposed in the southern and southeastern part of the massif and coincide with pronounced, high-amplitude magnetic anomalies attributed to elevated magnetite contents. Despite detailed petrological and geochemical studies, the structural continuation of these bodies toward the north and northwest beneath overlying nappes remains poorly constrained.

We address this problem through joint inversion of gravity and magnetic data, exploiting the characteristic properties of reduced bulk density and elevated magnetic susceptibility in serpentinized ultramafic rocks relative to the surrounding crystalline basement. We integrate newly acquired high-resolution airborne gravity and magnetic observations with vintage seismic reflection constraints and site-specific petrophysical measurements (density and magnetic susceptibility) conducted on samples collected from surface outcrops. We used topography-aware forward modelling and wavelet compression to efficiently handle dense airborne datasets. Geological and petrophysical information is incorporated through bound/interval constraints, while seismic reflectors provide structural guidance to steer the inversion toward geologically plausible geometries and reduce non-uniqueness.

Preliminary joint inversion results of serpentinites reproduce the observed magnetic anomaly patterns consistent with outcrop-based measurements. First joint gravity–magnetic models indicate that combining density and susceptibility constraints with structural guidance from vintage seismic reflection data improves the robustness of inferred serpentinite geometries compared to magnetic-only inversions, particularly with respect to thickness distribution and subsurface continuity beneath the massif.

The Münchberg Massif thus serves as a natural test site for developing and validating geophysical workflows to characterize potential natural hydrogen systems in settings where serpentinites are concealed beneath crystalline or sedimentary cover.

How to cite: Klitzke, P., Sobh, M., Ruppel, A., Bagge, M., Koglin, N., Hasch, M., Christiansen, R., Fazlikhani, H., Goldmann, J.-F., Heyde, I., and Löwer, A.: Imaging of Serpentinites beneath the Münchberg Massif (Germany) using Joint Gravity and Magnetic Inversion, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19008, https://doi.org/10.5194/egusphere-egu26-19008, 2026.