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Influence of Magnetic Fields on Precipitating Solar Wind Hydrogen at Mars
Journal article   Open access   Peer reviewed

Influence of Magnetic Fields on Precipitating Solar Wind Hydrogen at Mars

Sarah Henderson, Jasper Halekas, Zach Girazian, Jared Espley and Meredith Elrod
Geophysical research letters, Vol.49(12), e2022GL099114
06/28/2022
DOI: 10.1029/2022GL099114
PMCID: PMC9285465
PMID: 35860423
url
https://doi.org/10.1029/2022GL099114View
Published (Version of record) Open Access

Abstract

Solar wind protons can interact directly with the hydrogen corona of Mars through charge exchange, resulting in energetic neutral atoms (ENAs) able to penetrate deep into the upper atmosphere of Mars. ENAs can undergo multiple charge changing interactions, leading to an observable beam of penetrating protons in the upper atmosphere. We seek to characterize the behavior of these protons in the presence of magnetic fields using data collected by the Mars Atmosphere and Volatile EvolutioN spacecraft. We find that backscattered penetrating proton flux is enhanced in regions where the magnetic field strength is greater than 200 nT. We also find a strong correlation at CO2 column densities less than 5.5 x 10(14) cm(-2) between magnetic field strength and the observed backscattered and downward flux. We do not see significant changes in penetrating proton flux with magnetic field strengths on the order of 10 nT.
Geology Physical Sciences Geosciences, Multidisciplinary Science & Technology UIOWA OA Agreement

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