Upper mantle structure of Mars from InSight seismic data: Supplementary data

Amir Khan, , Martin Van Driel, Domenico Giardini, Philippe Lognonné, Henri Samuel, Nicholas C. Schmerr, Simon C. Stähler, Andrea C. Duran, , , Adrien Broquet, , John F. Clinton, Paul M. Davis, Mélanie Drilleau, Foivos Karakostas, Vedran Lekic, Scott M. McLennan, Ross R. Maguire, Chloé Michaut, Mark P. Panning, William T. Pike, Baptiste Pinot, Matthieu Plasman … & William B. Banerdt
We provide two seismic velocity models that are characteristic of the inverted families of models shown in Khan et al. (2021) (cf. Fig.2A). The blue and red models correspond to models with lithospheric thicknesses in the range 400-500 km and 500-600 km (cf. Fig.2B of Khan et al. (2021)), respectively. The models are here made available in digital format as named discontinuity (.nd) files. The four columns in each files are: depth in km, P-wave...
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