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Jul 21, 2021 -
Data from the article: Thickness and structure of the martian crust from InSight seismic data
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Jul 20, 2021
Khan, Amir; Ceylan, Savas; van Driel, Martin; Giardini, Domenico; Lognonné, Philippe; Samuel, Henri; Schmerr, Nicholas C.; Stähler, Simon C.; Duran, Andrea C.; Huang, Quancheng; Kim, Doyeon; Broquet, Adrien; Charalambous, Constantinos; Clinton, John F.; Davis, Paul M.; Drilleau, Mélanie; Karakostas, Foivos; Lekic, Vedran; McLennan, Scott M.; Maguire, Ross R.; Michaut, Chloé; Panning, Mark P.; Pike, William T.; Pinot, Baptiste; Plasman, Matthieu; Scholz, John-Robert; Widmer-Schnidrig, Rudolf; Spohn, Tilman; Smrekar, Suzanne E.; Banerdt, William B., 2021, "Upper mantle structure of Mars from InSight seismic data: Supplementary data", https://doi.org/10.18715/IPGP.2021.kpnr925g, IPGP Research Collection, V1
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.... |
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Jul 9, 2021
Stähler, Simon; Khan, Amir; Banerdt, W. Bruce; Lognonné, Philippe; Giardini, Domenico; Ceylan, Savas; Drilleau, Mélanie; Duran, A. Cecilia; Garcia, Raphaël F.; Huang, Quancheng; Kim, Doyeon; Lekic, Vedran; Samuel, Henri; Schimmel, Martin; Schmerr, Nicholas; Sollberger, David; Stutzmann, Éléonore; Xu, Zongbo; Antonangeli, Daniele; Charalambous, Constantinos; Davis, Paul M.; Irving, Jessica C.E.; Kawamura, Taichi; Knapmeyer, Martin; Maguire, Ross; Marusiak, Angela G.; Panning, Mark P.; Perrin, Clément; Plesa, Ana-Catalina; Rivoldini, Attilio; Schmelzbach, Cédric; Zenhäusern, Géraldine; Beucler, Éric; Clinton, John; Dahmen, Nikolaj; van Driel, Martin; Gudkova, Tamara; Horleston, Anna; Pike, W. Thomas; Plasman, Matthieu; Smrekar, Suzanne E., 2021, "Interior Models of Mars from inversion of seismic body waves", https://doi.org/10.18715/IPGP.2021.kpmqrnz8, IPGP Research Collection, V1
This dataset contains 300 seismic models of Mars compatible with seismic travel times of marsquakes observed until January 2021. The inversion is described in detail in Stähler et al. (2021): Seismic detection of the Martian Core, Science. See the description therein. The provide... |
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