• Calibration of the Heat Flow and Physical Properties Package (HP 3) for the InSight Mars Mission 

      Grott, M.ORCIDiD; Spohn, T.ORCIDiD; Knollenberg, J.; Krause, C.; Scharringhausen, M.; Wippermann, T.; Smrekar, S.E.ORCIDiD; Hudson, T.L.ORCIDiD; Banerdt, W.B. (Earth and Space Science, 2019)
      The (HP 3) of the InSight Mars mission is an instrument package to measure the Martian geothermal heat flow. The instrument's platinum resistance temperature sensors have been calibrated between −75 and +55 °C, and ...
    • Detection, Analysis, and Removal of Glitches From InSight's Seismic Data From Mars 

      Scholz, John‐Robert; Widmer‐Schnidrig, Rudolf; Davis, Paul; Lognonné, PhilippeORCIDiD; Pinot, Baptiste; Garcia, Raphaël F.ORCIDiD; Hurst, KennethORCIDiD; Pou, LaurentORCIDiD; Nimmo, FrancisORCIDiD; Barkaoui, SalmaORCIDiD; de Raucourt, Sébastien; Knapmeyer‐Endrun, BrigitteORCIDiD; Knapmeyer, MartinORCIDiD; Orhand‐Mainsant, Guénolé; Compaire, NicolasORCIDiD; Cuvier, Arthur; Beucler, ÉricORCIDiD; Bonnin, MickaëlORCIDiD; Joshi, RakshitORCIDiD; Sainton, Grégory; Stutzmann, EléonoreORCIDiD; Schimmel, MartinORCIDiD; Horleston, AnnaORCIDiD; Böse, Maren; Ceylan, SavasORCIDiD; Clinton, John; van Driel, Martin; Kawamura, Taichi; Khan, AmirORCIDiD; Stähler, Simon C.ORCIDiD; Giardini, DomenicoORCIDiD; Charalambous, ConstantinosORCIDiD; Stott, Alexander E.ORCIDiD; Pike, William T.; Christensen, Ulrich R.ORCIDiD; Banerdt, W. BruceORCIDiD (Earth and Space Science, 2020-10-30)
      The instrument package SEIS (Seismic Experiment for Internal Structure) with the three very broadband and three short‐period seismic sensors is installed on the surface on Mars as part of NASA's InSight Discovery mission. ...
    • 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 ...
    • The Global Seismic Moment Rate of Mars After Event S1222a 

      Knapmeyer, M.ORCIDiD; Stähler, S.ORCIDiD; Plesa, A.‐C.ORCIDiD; Ceylan, S.ORCIDiD; Charalambous, C.ORCIDiD; Clinton, J.; Dahmen, N.ORCIDiD; Durán, C.; Horleston, A.ORCIDiD; Kawamura, T.ORCIDiD; Kim, D.; Li, J.; Plasman, M.; Zenhäusern, G.ORCIDiD; Weber, R. C.ORCIDiD; Giardini, D.ORCIDiD; Panning, M. P.ORCIDiD; Lognonné, P.ORCIDiD; Banerdt, W. B.ORCIDiD (Geophysical Research Letters, 2023-04-06)
      The seismic activity of a planet can be described by the corner magnitude, events larger than which are extremely unlikely, and the seismic moment rate, the long‐term average of annual seismic moment release. Marsquake ...