Martian Electron Temperatures in the Subsolar Region: MAVEN Observations Compared to a One-Dimensional Model-Reference-Cited by-同舟云学术

Martian Electron Temperatures in the Subsolar Region: MAVEN Observations Compared to a One-Dimensional Model

Published:2018-07 Issue:7 Volume:123 Page:5960-5973
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Peterson W. K.¹^ORCID,Fowler C. M.¹^ORCID,Andersson L. A.¹^ORCID,Thiemann E. M. B.¹^ORCID,Jain S. K.¹^ORCID,Mayyasi M.²^ORCID,Esman T. M.³,Yelle R.³^ORCID,Benna M.⁴^ORCID,Espley J.⁴^ORCID

Affiliation:

1. LASP; University of Colorado Boulder; Boulder CO USA

2. Center for Space Physics; Boston University; Boston MA USA

3. Lunar and Planetary Laboratory; University of Arizona; Tucson AZ USA

4. NASA/Goddard Space Flight Center; Greenbelt MD USA

Funder

National Aeronautics and Space Administration

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1029/2018JA025406/fullpdf

Reference39 articles.

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4. Solar cycle variability of Mars dayside exospheric temperatures: Model evaluation of underlying thermal balances;Bougher;Geophysical Research Letters,2009

5. The role of the electron temperature on ion loss from Mars;Brecht;Journal of Geophysical Research: Space Physics,2017

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