Different Martian Crustal Seismic Velocities Across the Dichotomy Boundary From Multi‐Orbiting Surface Waves-Reference-Cited by-同舟云学术

Different Martian Crustal Seismic Velocities Across the Dichotomy Boundary From Multi‐Orbiting Surface Waves

Published:2023-01-10 Issue:1 Volume:50 Page:
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophysical Research Letters

Author:

Li Jiaqi¹^ORCID,Beghein Caroline¹^ORCID,Lognonné Philippe²^ORCID,McLennan Scott M.³^ORCID,Wieczorek Mark A.⁴^ORCID,Panning Mark P.⁵^ORCID,Knapmeyer‐Endrun Brigitte⁶,Davis Paul¹,Banerdt W. Bruce⁵^ORCID

Affiliation:

1. Department of Earth, Planetary, and Space Sciences University of California Los Angeles CA USA

2. CNRS Institut de physique du globe de Paris Université Paris Cité Paris France

3. Department of Geosciences Stony Brook University Stony Brook NY USA

4. Laboratoire Lagrange Observatoire de la Côte d’Azur CNRS Université Côte d’Azur Nice France

5. Jet Propulsion Laboratory California Institute of Technology Pasadena CA USA

6. Bensberg Observatory University of Cologne Bergisch Gladbach Germany

Funder

Agence Nationale de la Recherche

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2022GL101243

Reference61 articles.

1. The Borealis basin and the origin of the martian crustal dichotomy

2. Initial results from the InSight mission on Mars

3. Depth constraints on azimuthal anisotropy in the Great Basin from Rayleigh-wave phase velocity maps

4. Crustal Anisotropy in the Martian Lowlands From Surface Waves

5. Medusae Fossae Formation: New perspectives from Mars Global Surveyor

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