Now showing items 1-4 of 4

    • Assessing the Accuracy of 2‐D Planetary Evolution Models Against the 3‐D Sphere 

      Fleury, A.; Plesa, A.‐C.ORCIDiD; Hüttig, C.; Breuer, D.ORCIDiD (Geochemistry, Geophysics, Geosystems, 2024-02-07)

      Regardless of the steady increase of computing power during the last decades, numerical ...

    • Formation of Thermochemical Heterogeneities by Core‐Mantle Interaction 

      Stein, ClaudiaORCIDiD; Hansen, Ulrich (Journal of Geophysical Research: Solid Earth, 2023-02-17)
      Earth's core‐mantle boundary (CMB) shows a complex structure with various seismic anomalies such as the large low shear‐wave velocity provinces (LLSVPs) and ultra‐low velocity zones (ULVZs). As these structures are possibly ...
    • Mantle Convection Patterns Reveal the Mechanism of the Red Sea Rifting 

      Petrunin, A. G.ORCIDiD; Kaban, M. K.ORCIDiD; El Khrepy, S.ORCIDiD; Al-Arifi, N. (Tectonics, 2020)
      We present a new model of the stress state and present-day tectonics of the Red Sea Rift (RSR) based on an instantaneous geodynamic mantle flow model. The initial density and viscosity variations in the mantle are derived ...
    • 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 ...