logo seis
  • Accueil
  • Science
  • Produits SEIS
  • Interior Models of Mars from inversion of seismic body waves

Interior Models of Mars from inversion of seismic body waves

Interior Models of Mars from inversion of seismic body waves

Resource type
Dataset
Creators
Simon Stähler, Amir Khan, W. Bruce Banerdt, Philippe Lognonné, Domenico Giardini, Savas Ceylan, Mélanie Drilleau, A. Cecilia Duran, Raphaël F. Garcia, Quancheng Huang, Doyeon Kim, Vedran Lekic, Henri Samuel, Martin Schimmel, Nicholas Schmerr, David Sollberger, Éléonore Stutzmann, Zongbo Xu, Daniele Antonangeli, Constantinos Charalambous, Paul Davis, Jessica C.E. Irving, Taichi Kawamura, Martin Knapmeyer, Ross Maguire, Angela G. Marusiak, Mark P. Panning, Clément Perrin, Ana-Catalina Plesa, Attilio Rivoldini, Cédric Schmelzbach, Géraldine Zenhäusern, Éric Beucler, John Clinton, Nikolaj Dahmen, Martin Van Driel, Tamara Gudkova, Anna Horleston, W. Thomas Pike, Matthieu Plasman, Suzanne E. Smrekar
Publisher
IPGP Data Center
Publication Year
2021
Abstract
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..
Data and Citation
doi:10.18715/IPGP.2021.kpmqrnz8
logo IPGP bottom

Realized by IPGP (P. Labrot)

seis-support@ipgp.fr

 

 NASA JPL - Oxford University - Imperial College London - CNES - ISAE - MPS - IPGP - ETH