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JOURNAL OF GEOPHYSICAL RESEARCH,
VOL. 83, NO. A3,
PAGES 1172–1174,
1978
Electron Cooling by Excitation of Carbon Dioxide
Michael A. Morrison
Theoretical Division T-12, Los Alamos Scientific Laboratory, Los Alamos, New Mexico 87545
Arthur E. Greene
Theoretical Division T-12, Los Alamos Scientific Laboratory, Los Alamos, New Mexico 87545
Abstract
The cooling of a heated electron gas by electron impact excitation of CO2 is believed to be an important process in the neutral atmospheres of Mars and Venus. Electron energy loss rates are calculated
for a variety of excitation processes as a function of electron temperature at a CO2 gas temperature of 200 K. Vibrational excitation is found to be the most efficient cooling mechanism for the range of electron
temperatures studied. The contributions of various vibrational energy loss processes to electron cooling are discussed.
Received 18
July
1977;
accepted 30
October
1977.
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Citation: Morrison, M. A., and A. E. Greene
(1978),
Electron Cooling by Excitation of Carbon Dioxide,
J. Geophys. Res.,
83(A3),
1172–1174.
Copyright 1978 by the American Geophysical Union.
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