Article (Scientific journals)
OGO-4 observations of the ultraviolet auroral spectrum
Gérard, Jean-Claude; Barth, C. A.
1976In Planetary and Space Science, 24, p. 1059-1063
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Keywords :
ATOMIC SPECTRA; AURORA; MOLECULAR SPECTRA; NITRIC OXIDE; SATELLITE OBSERVATION; ULTRAVIOLET SPECTRA; GAMMA RAYS; HYDROGEN ATOMS; MOLECULAR EXCITATION; NITROGEN; OGO-4; OXYGEN
Abstract :
[en] Auroral ultraviolet spectra in the range from 1200 to 3200 A have been obtained by the spectrometer on board the OGO-4 satellite. Emissions of N2, H, O, and N are readily identified. Atomic and molecular intensities are deduced from the comparison with a synthetic spectrum and compare reasonably well with some previous measurements and calculations. A feature at 2150 A is assigned to the (1-0) NO gamma band. Taking into consideration the various excitation mechanisms of NO(A2 Sigma), it is proposed that energy transfer from N2 metastable molecules to oxygen accounts for the excitation of the NO gamma bands. In particular, it is suggested that the resonant reaction between O2 and highly metastable N2 molecules may be a major source of NO(A2 Sigma).
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Gérard, Jean-Claude  ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Labo de physique atmosphérique et planétaire (LPAP)
Barth, C. A.;  Colorado, University, Boulder, Colo.
Language :
English
Title :
OGO-4 observations of the ultraviolet auroral spectrum
Publication date :
01 November 1976
Journal title :
Planetary and Space Science
ISSN :
0032-0633
Publisher :
Pergamon Press - An Imprint of Elsevier Science, Oxford, United Kingdom
Volume :
24
Pages :
1059-1063
Peer reviewed :
Peer Reviewed verified by ORBi
Available on ORBi :
since 31 October 2009

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