• Seismic Velocity Variations in a 3D Martian Mantle: Implications for the InSight Measurements 

      Plesa, A.‐C.ORCIDiD; Bozdağ, E.ORCIDiD; Rivoldini, A.ORCIDiD; Knapmeyer, M.ORCIDiD; McLennan, S. M.ORCIDiD; Padovan, S.ORCIDiD; Tosi, N.ORCIDiD; Breuer, D.ORCIDiD; Peter, D.ORCIDiD; Stähler, S.ORCIDiD; Wieczorek, M. A.ORCIDiD; van Driel, M.ORCIDiD; Khan, A.ORCIDiD; Spohn, T.ORCIDiD (Journal of Geophysical Research: Planets, 2021-06-17)
      We use a large data set of 3D thermal evolution models to predict the distribution of present‐day seismic velocities in the Martian interior. Our models show a difference between maximum and minimum S wave velocity of up ...
    • Toward Constraining Mars' Thermal Evolution Using Machine Learning 

      Agarwal, S.ORCIDiD; Tosi, N.ORCIDiD; Kessel, P.; Padovan, S.ORCIDiD; Breuer, D.ORCIDiD; Montavon, G. (Earth and Space Science, 2021-04-23)
      The thermal and convective evolution of terrestrial planets like Mars is governed by a number of initial conditions and parameters, which are poorly constrained. We use Mixture Density Networks (MDN) to invert various sets ...