Electron energetics in the Martian dayside ionosphere: Model comparisons with MAVEN data - Archive ouverte HAL Access content directly
Journal Articles Journal of Geophysical Research: Space Physics Year : 2016

Electron energetics in the Martian dayside ionosphere: Model comparisons with MAVEN data

, , , , (1) , , , , , , , , ,
1
Shotaro Sakai
Laila Andersson
  • Function : Author
Thomas E. Cravens
  • Function : Author
David L. Mitchell
  • Function : Author
Ali Rahmati
Christopher M. Fowler
  • Function : Author
Stephen W. Bougher
  • Function : Author
Edward M. B. Thiemann
  • Function : Author
Francis G. Eparvier
  • Function : Author
Juan M. Fontenla
  • Function : Author
Paul R. Mahaffy
  • Function : Author
John E. P. Connerney
  • Function : Author
Bruce M. Jakosky
  • Function : Author

Abstract

This paper presents a study of the energetics of the dayside ionosphere of Mars using models and data from several instruments on board the Mars Atmosphere and Volatile EvolutioN spacecraft. In particular, calculated photoelectron fluxes are compared with suprathermal electron fluxes measured by the Solar Wind Electron Analyzer, and calculated electron temperatures are compared with temperatures measured by the Langmuir Probe and Waves experiment. The major heat source for the thermal electrons is Coulomb heating from the suprathermal electron population, and cooling due to collisional rotational and vibrational CO2 dominates the energy loss. The models used in this study were largely able to reproduce the observed high topside ionosphere electron temperatures (e.g., 3000 K at 300 km altitude) without using a topside heat flux when magnetic field topologies consistent with the measured magnetic field were adopted. Magnetic topology affects both suprathermal electron transport and thermal electron heat conduction. The effects of using two different solar irradiance models were also investigated. In particular, photoelectron fluxes and electron temperatures found using the Heliospheric Environment Solar Spectrum Radiation irradiance were higher than those with the Flare Irradiance Spectrum Model-Mars. The electron temperature is shown to affect the O2+ dissociative recombination rate coefficient, which in turn affects photochemical escape of oxygen from Mars.
Fichier principal
Vignette du fichier
JGR Space Physics - 2016 - Sakai - Electron energetics in the Martian dayside ionosphere Model comparisons with MAVEN data.pdf (15.2 Mo) Télécharger le fichier
Origin : Publisher files allowed on an open archive

Dates and versions

insu-03669462 , version 1 (17-05-2022)

Licence

Copyright

Identifiers

Cite

Shotaro Sakai, Laila Andersson, Thomas E. Cravens, David L. Mitchell, Christian Mazelle, et al.. Electron energetics in the Martian dayside ionosphere: Model comparisons with MAVEN data. Journal of Geophysical Research: Space Physics, 2016, 121, pp.7049-7066. ⟨10.1002/2016JA022782⟩. ⟨insu-03669462⟩
17 View
3 Download

Altmetric

Share

Gmail Facebook Twitter LinkedIn More