Properties of Plasma Waves Observed Upstream From Mars-Reference-Cited by-同舟云学术

Properties of Plasma Waves Observed Upstream From Mars

Published:2020-09 Issue:9 Volume:125 Page:
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Halekas J. S.¹^ORCID,Ruhunusiri S.¹^ORCID,Vaisberg O. L.²^ORCID,Harada Y.³^ORCID,Espley J. R.⁴,Mitchell D. L.⁵^ORCID,Mazelle C.⁶^ORCID,Romanelli N.⁴⁷^ORCID,DiBraccio G. A.⁴^ORCID,Brain D. A.⁸^ORCID

Affiliation:

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

2. Space Research Institute Russian Academy of Sciences Moscow Russia

3. Department of Geophysics Kyoto University Kyoto Japan

4. NASA Goddard Space Flight Center Greenbelt MD USA

5. Space Sciences Laboratory University of California Berkeley CA USA

6. IRAP University of Toulouse Toulouse France

7. CRESST II University of Maryland Baltimore MD USA

8. Laboratory for Atmospheric and Space Physics University of Colorado Boulder CO USA

Funder

National Aeronautics and Space Administration

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2020JA028221

Reference73 articles.

1. Mariner 6 and 7 Ultraviolet Spectrometer Experiment: Analysis of hydrogen Lyman-alpha data

2. Theory of generation of bow‐shock‐associated hydromagnetic waves in the upstream interplanetary medium;Barnes A.;Cosmic Electrodynamics,1970

3. Temporal variability of waves at the proton cyclotron frequency upstream from Mars: Implications for Mars distant hydrogen exosphere

4. A strong seasonal dependence in the Martian hydrogen exosphere

5. Observations of low-frequency electromagnetic plasma waves upstream from the Martian shock

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