Modelling the effects of 3D shallow scatterers and atmospheric sources on Martian seismic signals at high frequencies
Tarje Nissen-Meyer1, Benjamin Fernando2, Kuangdai Leng2, Nicholas C Schmerr3, Mark P Panning4, Eleonore Stutzmann5, Ludovic Margerin6, Nobuaki Fuji5, Renee C Weber7, William Bruce Banerdt8, Domenico Giardini9, Philippe Henri Lognonné5 and William T Pike10, (1)University of Oxford, Department of Earth Sciences, Oxford, United Kingdom, (2)University of Oxford, Oxford, United Kingdom, (3)University of Maryland College Park, Geology, College Park, MD, United States, (4)Univ of FL-Geological Sciences, Gainesville, FL, United States, (5)Université de Paris, Institut de physique du globe de Paris, CNRS, Paris, France, (6)Observatory Midi-Pyrenees, Toulouse, France, (7)NASA/NSSTC, Huntsville, AL, United States, (8)Jet Propulsion Laboratory, Pasadena, CA, United States, (9)ETH Zurich, Zurich, Switzerland, (10)Imperial College London, London, SW7, United Kingdom