Micro‐Scale Plasma Instabilities in the Interaction Region of the Solar Wind and the Martian Upper Atmosphere-Reference-Cited by-同舟云学术

Micro‐Scale Plasma Instabilities in the Interaction Region of the Solar Wind and the Martian Upper Atmosphere

Published:2022-05 Issue:5 Volume:127 Page:
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:JGR Space Physics

Author:

Akbari Hassanali¹^ORCID,Newman David²^ORCID,Fowler Christopher³^ORCID,Pfaff Robert¹^ORCID,Andersson Laila⁴^ORCID,Malaspina David⁴^ORCID,Schwartz Steven⁴^ORCID,Ergun Robert⁴^ORCID,McFadden James⁵,Mitchell David⁵^ORCID,Halekas Jasper⁶^ORCID,Rowland Douglas¹

Affiliation:

1. NASA Goddard Space Flight Center Greenbelt MD USA

2. Center for Integrated Plasma Studies University of Colorado Boulder Boulder CO USA

3. Department of Physics and Astronomy West Virginia University Morgantown VW USA

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

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

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

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2022JA030591

Reference38 articles.

1. The Langmuir Probe and Waves (LPW) Instrument for MAVEN

2. The Induced Magnetospheres of Mars, Venus, and Titan

3. Solar Wind Induced Waves in the Skies of Mars: Ionospheric Compression, Energization, and Escape Resulting From the Impact of Ultralow Frequency Magnetosonic Waves Generated Upstream of the Martian Bow Shock

4. The MAVEN Magnetic Field Investigation

5. Interaction of the Solar Wind with Unmagnetized Planets

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