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Evidence of electron impact ionization in the magnetic pileup boundary of Mars
Author(s) -
Crider D.,
Cloutier P.,
Law C.,
Walker P.,
Chen Y.,
Acuña M.,
Connerney J.,
Mitchell D.,
Lin R.,
Anderson K.,
Carlson C.,
McFadden J.,
Rème H.,
Mazelle C.,
d'Uston C.,
Sauvaud J.,
Vignes D.,
Brain D.,
Ness N.
Publication year - 2000
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/1999gl003625
Subject(s) - ionization , electron ionization , electron , physics , mars exploration program , atomic physics , bow shock (aerodynamics) , computational physics , shock wave , astrobiology , ion , nuclear physics , thermodynamics , quantum mechanics
A sharp decline in electron fluxes is observed in the Mars Global Surveyor Electron Reflectometer data in conjunction with the magnetic pileup boundary. We examine the characteristics of the evolution of the electron distribution function for one orbit. We determine that the spectra can best be explained by electron impact ionization of oxygen and hydrogen. To reproduce the observed spectral evolution, we construct a model of the effects of electron impact ionization on the electron distribution function as a flow element encounters the neutral atmosphere. Using the observed post‐shock electron distribution function, we are able to reproduce the observed flux attenuation. We conclude that electron impact ionization is the physical mechanism responsible for the spectral feature.