Observations and Modeling of the Mars Low-Altitude Ionospheric Response to the 10 September 2017 X-Class Solar Flare

Author:

Xu Shaosui1ORCID,Thiemann Ed2ORCID,Mitchell David1ORCID,Eparvier Frank2ORCID,Pawlowski David3,Benna Mehdi4ORCID,Andersson Laila2ORCID,Liemohn Michael W.5ORCID,Bougher Stephen5ORCID,Mazelle Christian6ORCID

Affiliation:

1. Space Sciences Laboratory; University of California; Berkeley CA USA

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

3. Physics Department; Eastern Michigan University; Ypsilanti MI USA

4. NASA Goddard Space Flight Center; Greenbelt MD USA

5. Department of Climate and Space Sciences and Engineering; University of Michigan; Ann Arbor MI USA

6. IRAP; CNRS-University of Toulouse-UPS-CNES; Toulouse France

Funder

National Aeronautics and Space Administration

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Reference51 articles.

1. The Langmuir Probe and Waves (LPW) instrument for MAVEN;Andersson;Space Science Reviews,2015

2. Mars global surveyor radio science electron density profiles: Neutral atmosphere implications;Bougher;Geophysical Research Letters,2001

3. Mars Global Ionosphere-Thermosphere Model: Solar cycle, seasonal, and diurnal variations of the Mars upper atmosphere;Bougher;Journal of Geophysical Research: Planets,2015

4. The absorption and dissociative or ionizing effect of monochromatic radiation in an atmosphere on a rotating Earth;Chapman;Proceedings of the Physical Society,1931a

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