Simulating Impacts of Electron Precipitation on Mars' Nightside Ionosphere With an Empirical Model

Abstract With the aim of improving global simulations of the Martian ionosphere, we present an empirical model of 137 electron impact processes—including ionization, dissociation, and excitation—on the nightside of Mars, based on MAVEN in situ data collected between 2014 and 2019. The empirical model demonstrates the significant impact magnetic field conditions have on nightside ionization rates, with different magnetic topologies reversing trends previously seen in ionization dependence on magnetic field strength: closed field lines on the nightside show a decrease in ionization with stronger fields, while topologies where field lines connect to a source of plasma at one or both ends show an increase of ionization with stronger fields. This empirical model is coupled with magnetic fields from MHD simulations of the Martian magnetosphere, as input to the PCM‐Mars and M‐GITM thermosphere‐ionosphere models, to provide a source of ionization on the nightside. Finally, we present new simulations of the global ionosphere with ionization sources on both the dayside and, for the first time, the nightside.

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Publication Details

Journal
Journal of Geophysical Research Planets
Published
2025-03-27
DOI
https://doi.org/10.1029/2025je008953
Citations
1
Primary Topic
Planetary Science and Exploration
Type
article
Field-Weighted Citation Impact
1.15

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article

Simulating Impacts of Electron Precipitation on Mars' Nightside Ionosphere With an Empirical Model

Francisco González‐Galindo, Shannon Curry, J. S. Halekas, M. Marquette et al.
1 citations
Journal of Geophysical Research Planets
Planetary Science and Exploration
1.15
article

Simulating Impacts of Electron Precipitation on Mars' Nightside Ionosphere With an Empirical Model

Francisco González‐Galindo, Shannon Curry, J. S. Halekas, M. Marquette, M. K. Elrod, R. J. Lillis, D. J. Pawlowski, J. R. Espley, M. Benna, J. Gruesbeck, Yingjuan Ma, Jean‐Yves Chaufray, D. L. Mitchell
article en
1 citations

Abstract

Abstract With the aim of improving global simulations of the Martian ionosphere, we present an empirical model of 137 electron impact processes—including ionization, dissociation, and excitation—on the nightside of Mars, based on MAVEN in situ data collected between 2014 and 2019. The empirical model demonstrates the significant impact magnetic field conditions have on nightside ionization rates, with different magnetic topologies reversing trends previously seen in ionization dependence on magnetic field strength: closed field lines on the nightside show a decrease in ionization with stronger fields, while topologies where field lines connect to a source of plasma at one or both ends show an increase of ionization with stronger fields. This empirical model is coupled with magnetic fields from MHD simulations of the Martian magnetosphere, as input to the PCM‐Mars and M‐GITM thermosphere‐ionosphere models, to provide a source of ionization on the nightside. Finally, we present new simulations of the global ionosphere with ionization sources on both the dayside and, for the first time, the nightside.

Journal of Geophysical Research PlanetsVol. 130(4)
University of Iowa (US), Planetary Science Institute (US), Goddard Space Flight Center (US), Eastern Michigan University (US), University of California, Los Angeles (US), University of Colorado Boulder (US), Laboratory for Atmospheric and Space Physics (US), Laboratoire atmosphères, milieux, observations spatiales (FR), Instituto de Astrofísica de Andalucía (ES), University of Maryland, College Park (US), University of Maryland, Baltimore County (US), University of California, Berkeley (US)
National Aeronautics and Space Administration, Centre National d’Etudes Spatiales, Nuclear Safety and Security Commission, Goddard Space Flight Center, Science Mission Directorate
Openalex Percentile: Top 20%
Planetary Science and Exploration
1.15
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