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Largest Electron Differential Energy Flux Observed at Mars, 2004-2016
Frahm, R.A.; Winninham, J.D.; Coates, A.J. et al.
2017International Mars Aeronomy Conference
 

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Keywords :
Mars; electron flux; précipitation; ASPERA; Venus
Abstract :
[en] The shape of the largest DEF electron spectrum is similar at Mars and Venus. The shape of the largest DEF electron spectra at Mars and Venus is similar to the electron spectrum detected during the times SPICAM detects “auroral” enhanced signatures. Since the magnetic field at Mars is chaotic, the largest DEF electron spectrum could be magnetically directed from the dayside to the nightside where it could precipitate causing the same “auroral” signature seen by SPICAM.
Research center :
LPAP
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Frahm, R.A.
Winninham, J.D.
Coates, A.J.
Gérard, Jean-Claude  ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Département d'astrophys., géophysique et océanographie (AGO)
Holström, H.
Barabash, S.
Language :
English
Title :
Largest Electron Differential Energy Flux Observed at Mars, 2004-2016
Publication date :
17 May 2017
Event name :
International Mars Aeronomy Conference
Event organizer :
University of Colorado
Event place :
Boulder, United States
Event date :
15-19 mai 2017
Audience :
International
Funders :
BELSPO - SPP Politique scientifique - Service Public Fédéral de Programmation Politique scientifique
Available on ORBi :
since 31 December 2017

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