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  • Authors: J Rojas-Sandoval; P Acevedo-Rodríguez;
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  • Authors: J Rojas-Sandoval; N Pasiecznik;
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  • Authors: Eduardo A. Ventosa-Febles;
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  • Authors: Stähler, Simon; Khan, Amir; Banerdt, W. Bruce; Lognonné, Philippe; +37 Authors

    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 provided zip file contains 100 models each of the "geophysical", "geodynamical" and "seismic" inversion. All model files are provided in the nd format of TauP. For compatibility reasons, each model has a small inner core. This is not a feature resolved by the inversion.

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  • Authors: Ling Cao;
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  • Authors: Manuel Angel Duenas-Lopez;
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  • Authors: Marianne Jennifer Datiles; Pedro Acevedo-Rodríguez;
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  • Authors: Stanley Gehrt;
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  • Authors: J Rojas-Sandoval; P Acevedo-Rodríguez;
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  • Authors: Ian Popay;
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1,531 Research products
  • Authors: J Rojas-Sandoval; P Acevedo-Rodríguez;
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  • Authors: J Rojas-Sandoval; N Pasiecznik;
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  • Authors: Eduardo A. Ventosa-Febles;
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  • Authors: Stähler, Simon; Khan, Amir; Banerdt, W. Bruce; Lognonné, Philippe; +37 Authors

    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 provided zip file contains 100 models each of the "geophysical", "geodynamical" and "seismic" inversion. All model files are provided in the nd format of TauP. For compatibility reasons, each model has a small inner core. This is not a feature resolved by the inversion.

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  • Authors: Ling Cao;
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  • Authors: Manuel Angel Duenas-Lopez;
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  • Authors: Marianne Jennifer Datiles; Pedro Acevedo-Rodríguez;
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