Ionospheric-electron heating by dissociative recombination

It is shown that the loss of ionospheric electrons by dissociative recombination effectively heats the electron gas at a rate which is a few per cent of the main heating rate due to photoelectrons but which exceeds some of the rates for minor cooling processes frequently included in energy-balance s...

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Veröffentlicht in:Planetary and space science 1974-01, Vol.22 (9), p.1343-1346
Hauptverfasser: Hamlin, D.A., Myers, B.F.
Format: Artikel
Sprache:eng
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Zusammenfassung:It is shown that the loss of ionospheric electrons by dissociative recombination effectively heats the electron gas at a rate which is a few per cent of the main heating rate due to photoelectrons but which exceeds some of the rates for minor cooling processes frequently included in energy-balance studies.
ISSN:0032-0633
1873-5088
DOI:10.1016/0032-0633(74)90056-7