Preprints
https://doi.org/10.5194/se-2020-145
https://doi.org/10.5194/se-2020-145

  16 Sep 2020

16 Sep 2020

Review status: a revised version of this preprint was accepted for the journal SE and is expected to appear here in due course.

Gravity Effect of Alpine Slab Segments Based on Geophysical and Petrological Modelling

Maximilian Lowe1, Jörg Ebbing1, Amr El-Sharkawy1,2, and Thomas Meier1 Maximilian Lowe et al.
  • 1Institute for Geosciences, Kiel University, Germany
  • 2National Research Institute of Astronomy and Geophysics, 11421, Helwan, Cairo, Egypt

Abstract. We study the potential gravity effect of suggested slab configurations beneath the Alpine mountain belt. The opposing slab configurations are based on seismic crustal thickness estimates and high-resolution upper mantle tomographies. Direct conversion of upper mantle seismic velocities to densities results in a gravity response that reflects results in a gravity field that may be interpreted as related to the effect of subducting lithosphere, however the different contributing slab segments cannot be clearly identified. Therefore, we define the geometry of the upper slab interface by using the crustal thickness at 40 km depth as upper starting point. Based on seismic tomography, the slab interface is followed down to 200 km depth. We define two alternative models for the slab configuration in the Alpine region in line with recently proposed hypotheses. The gravity effect of these alternative models is calculated for (i) a simple constant density distribution in the slab and (ii) accounting for compositional and thermal variations with depth. The forward calculations predict a gravity effect of the slab up to 40 mGal and significant differences in the pattern of the anomalies.

Maximilian Lowe et al.

 
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Status: closed
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Status: closed
Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
Printer-friendly Version - Printer-friendly version Supplement - Supplement

Maximilian Lowe et al.

Maximilian Lowe et al.

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