CONSTRAINTS ON THE DEPTH OF MARTIAN MANTLE TRANSITION ZONE FROM TRIPLICATED WAVEFORMS.
WAVEFORMS. Q. Huang, N. C. Schmerr, S. D. King, A. Rivoldini, A.-C. Plesa, H. Samuel, D. Kim, R. R. Maguire, F. Karakostas, V. Lekić, M. Collinet, R. Myhill, D. Antonangeli, M. Drilleau, M. Bystricky, C. Bollinger, C. Michaut, T. Gudkova, J. C.E. Irving, B. Fernando, K. Leng, T. Nissen-Meyer, F. Bejina, E. Bozdag, C. Beghein, L. Waszek, N. C. Siersch, J.-R. Scholz, P. M. Davis, P. Lognonné, B. Pinot, R. Widmer-Schnidrig, M. P. Panning, S. E. Smrekar, T. Spohn, D. Giardini, W. B. Banerdt; University of Maryland, Colorado School of Mines, Virginia Tech, Royal Observatory of Belgium, Institute of Planetary Research, German Aerospace Center (DLR), Université de Paris, Institut de Physique du Globe de Paris, Istituto Nazionale di Geofisica e Vulcanologia, Sezione di Bologna, University of Bristol, Sorbonne Université, Institut Supérieur de l'Aéronautique et de l'Espace SUPAERO, Institut de Recherche en Astrophysique et Planétologie, Université Toulouse III Paul Sabatier, 12 Université de Lyon, Schmidt Institute of Physics of the Earth RAS, University of Oxford, UCLA, James Cook University, Max Planck Institute for Solar System Research, Black Forest Observatory, Stuttgart University, JPL, ETH Zurich