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.

DOI: doi:10.18715/IPGP.2021.kpnr925g
Datacite: [ search ]
Citation: Khan, A., Savas Ceylan, Van Driel, M., Giardini, D., Lognonné, P., Samuel, H., Schmerr, N. C., Stähler, S. C., Duran, A. C., Quancheng Huang, Doyeon Kim, Broquet, A., Constantinos Charalambous, Clinton, J. F., Davis, P. M., Drilleau, M., Karakostas, F., Lekic, V., McLennan, S. M., … Banerdt, W. B. (2021). Upper mantle structure of Mars from InSight seismic data: Supplementary data [Data set]. IPGP Data Center. https://doi.org/10.18715/IPGP.2021.kpnr925g