On the Detectability and Use of Normal Modes for Determining Interior Structure of Mars

Felix Bissig (1) , Amir Khan (1) , Martin van Driel , Simon C Stähler (2) , Domenico Giardini (2) , Mark P Panning (3) , Melanie Drilleau (4) , Philippe Lognonné (5) , Tamara Gudkova (6) , Vladimir Zharkov (6) , Ana-Catalina Plesa (7) , William B. Banerdt (8)

1 Swiss Fed Inst Technol, Inst Geophys, Sonneggstr 5, CH-8092 Zurich, Switzerland
2 Institute of Geophysics [ETH Zürich]
3 JPL - Jet Propulsion Laboratory
4 IPGP - Institut de Physique du Globe de Paris
5 IPGP - Institut de Physique du Globe de Paris
6 Schmidt Institute of Physics of the Earth of the Russian Academy of Sciences (IPE RAS), Bolshaya Gruzinskaya Str. 10-1, 123242 Moscow, Russia
7 DLR Institut für Planetenforschung
8 Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA

Keywords: Author Keywords:Mars; Seismology; Normal modes; Interior structure; Inverse problems KeyWords Plus:FREE OSCILLATIONS; INSIGHT MISSION; SINGLE-STATION; TORSIONAL OSCILLATIONS; MARTIAN SEISMICITY; BULK COMPOSITION; MANTLE MINERALS; LUNAR INTERIOR; WAVE-FORMS; EARTH

Domains: Sciences of the Universe [physics]; Astrophysics [astro-ph]; Earth and Planetary Astrophysics [astro-ph.EP]

Felix Bissig, Amir Khan, Martin van Driel, Simon C Stähler, Domenico Giardini, et al.. On the Detectability and Use of Normal Modes for Determining Interior Structure of Mars. Space Science Reviews, 2018, 214 (8), ⟨10.1007/s11214-018-0547-9⟩. ⟨insu-02546649⟩