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

Resource type

Dataset

Creators

Amir Khan, Savas Ceylan, Martin van Driel, Domenico Giardini, Philippe Lognonné, Henri Samuel, Nicholas C. Schmerr, Simon C. Stähler, Andrea C. Duran, Quancheng Huang, Doyeon Kim, Adrien Broquet, Constantinos Charalambous, 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, John-Robert Scholz, Rudolf Widmer-Schnidrig, Tilman Spohn, Suzanne E. Smrekar, William B. Banerdt

Publisher

IPGP Data Center

Publication Year

2021

Abstract

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 velocity in km/s, S-wave velocity in km/s, and density in kg/m^3. When using or displaying the models, please cite: Khan, A., et al., Upper mantle structure of Mars from InSight seismic data, Science, 10.1126/science.abf2966, 2021.

Data and Citation

doi:10.18715/IPGP.2021.kpnr925g