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Detailed Reference Information |
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. and Ness, N. (2000). Evidence of electron impact ionization in the magnetic pileup boundary of Mars. Geophysical Research Letters 27: doi: 10.1029/1999GL003625. issn: 0094-8276. |
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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. ¿ 2000 American Geophysical Union |
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Abstract |
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Keywords
Planetology, Solid Surface Planets, Interactions with particles and fields, Planetology, Solar System Objects, Mars, Space Plasma Physics, Ionization processes |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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