Solar wind modulation of the Martian ionosphere observed by Mars Global Surveyor

Electron density profiles in the Martian ionosphere observed by the radio occultation experiment on board Mars Global Surveyor have been analyzed to determine if the densities are influenced by the solar wind. Evidence is presented that the altitude of the maximum ionospheric electron density sh...

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Main Authors: J.-S. Wang, E. Nielsen
Format: Article
Language:English
Published: Copernicus Publications 2004-06-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/22/2277/2004/angeo-22-2277-2004.pdf
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author J.-S. Wang
J.-S. Wang
E. Nielsen
author_facet J.-S. Wang
J.-S. Wang
E. Nielsen
author_sort J.-S. Wang
collection DOAJ
description Electron density profiles in the Martian ionosphere observed by the radio occultation experiment on board Mars Global Surveyor have been analyzed to determine if the densities are influenced by the solar wind. Evidence is presented that the altitude of the maximum ionospheric electron density shows a positive correlation to the energetic proton flux in the solar wind. The solar wind modulation of the Martian ionosphere can be attributed to heating of the neutral atmosphere by the solar wind energetic proton precipitation. The modulation is observed to be most prominent at high solar zenith angles. It is argued that this is consistent with the proposed modulation mechanism.
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spelling doaj.art-8c51cf4872aa41d78d72dfe9504dc77f2022-12-22T00:58:01ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762004-06-01222277228110.5194/angeo-22-2277-2004Solar wind modulation of the Martian ionosphere observed by Mars Global SurveyorJ.-S. Wang0J.-S. Wang1E. Nielsen2Max-Planck-Institut für Aeronomie, 37191 Katlenburg-Lindau, GermanySchool of Earth and Space Sciences, Peking University, Beijing 100871, ChinaMax-Planck-Institut für Aeronomie, 37191 Katlenburg-Lindau, GermanyElectron density profiles in the Martian ionosphere observed by the radio occultation experiment on board Mars Global Surveyor have been analyzed to determine if the densities are influenced by the solar wind. Evidence is presented that the altitude of the maximum ionospheric electron density shows a positive correlation to the energetic proton flux in the solar wind. The solar wind modulation of the Martian ionosphere can be attributed to heating of the neutral atmosphere by the solar wind energetic proton precipitation. The modulation is observed to be most prominent at high solar zenith angles. It is argued that this is consistent with the proposed modulation mechanism.https://www.ann-geophys.net/22/2277/2004/angeo-22-2277-2004.pdf
spellingShingle J.-S. Wang
J.-S. Wang
E. Nielsen
Solar wind modulation of the Martian ionosphere observed by Mars Global Surveyor
Annales Geophysicae
title Solar wind modulation of the Martian ionosphere observed by Mars Global Surveyor
title_full Solar wind modulation of the Martian ionosphere observed by Mars Global Surveyor
title_fullStr Solar wind modulation of the Martian ionosphere observed by Mars Global Surveyor
title_full_unstemmed Solar wind modulation of the Martian ionosphere observed by Mars Global Surveyor
title_short Solar wind modulation of the Martian ionosphere observed by Mars Global Surveyor
title_sort solar wind modulation of the martian ionosphere observed by mars global surveyor
url https://www.ann-geophys.net/22/2277/2004/angeo-22-2277-2004.pdf
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