The shallow structure of Mars at the InSight landing site from inversion of ambient vibrations

The shallow structure of Mars at the InSight landing site from inversion of ambient vibrations

We invert Rayleigh wave ellipticity curves extracted from ambient seismic vibrations at the InSight landing site to resolve, for the first time on Mars, the shallow subsurface to around 200 m depth. While our seismic velocity model is largely consistent with the expected stacks of lava flows, we fin...

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Autores principales: M. Hobiger, M. Hallo, C. Schmelzbach, S. C. Stähler, D. Fäh, D. Giardini, M. Golombek, J. Clinton, N. Dahmen, G. Zenhäusern, B. Knapmeyer-Endrun, S. Carrasco, C. Charalambous, K. Hurst, S. Kedar, W. B. Banerdt
Formato: article
Lenguaje:EN
Publicado: Nature Portfolio 2021
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Acceso en línea:https://doaj.org/article/981e593d21b04915984d2f1606bda1f5
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https://doaj.org/article/981e593d21b04915984d2f1606bda1f5

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