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

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.