MAVEN Proton Observations Near the Martian Moon Phobos: Does Phobos Backscatter Solar Wind Protons?-Reference-Cited by-同舟云学术

MAVEN Proton Observations Near the Martian Moon Phobos: Does Phobos Backscatter Solar Wind Protons?

Published:2022-12 Issue:23 Volume:49 Page:
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophysical Research Letters

Author:

Deniau A.¹²^ORCID,Nénon Q.¹^ORCID,André N.¹^ORCID,Mazelle C.¹^ORCID,Rahmati A.³^ORCID,Fowler C. M.⁴^ORCID,Poppe A. R.³^ORCID,McFadden J. P.³,Halekas J. S.⁵^ORCID,Penou E.¹

Affiliation:

1. Institut de Recherche en Astrophysique et Planétologie (IRAP) CNRS‐Université Toulouse III‐CNES Toulouse France

2. ISAE‐Supaéro Toulouse France

3. Space Sciences Laboratory University of California at Berkeley Berkeley CA USA

4. Department of Physics and Astronomy West Virginia University Morgantown WV USA

5. Department of Physics and Astronomy University of Iowa Iowa City IA USA

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2022GL101014

Reference37 articles.

1. AMDA. (2022a).Magnetic field vector in MSO coordinates observed by MAVEN‐MAG with a 1 second resolution[Dataset].Automated Multi‐Dataset Analysis (AMDA). Retrieved fromhttp://amda.irap.omp.eu

2. AMDA. (2022b).MAVEN position in MSO coordinates with a 1 second resolution[Dataset].Automated Multi‐Dataset Analysis (AMDA). Retrieved fromhttp://amda.irap.omp.eu

3. AMDA. (2022c).Phobos position in MSO coordinates with a 1 second resolution[Dataset].Automated Multi‐Dataset Analysis (AMDA). Retrieved fromhttp://amda.irap.omp.eu

4. AMDA. (2022d).Velocity of the solar wind in MSO coordinates computed from MAVEN‐SWIA observations with a 4 second resolution[Dataset].Automated Multi‐Dataset Analysis (AMDA). Retrieved fromhttp://amda.irap.omp.eu

5. Picked-up protons near Mars: Phobos observations

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