Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/54958
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dc.contributor.authorCampbell, Laurenceen
dc.contributor.authorBrunger, Michael J.en
dc.contributor.authorPetrovic, Z. L.en
dc.contributor.authorJelisavcic, M.en
dc.contributor.authorPanajotovic, R.en
dc.contributor.authorBuckman, Stephen J.en
dc.date.issued2004en
dc.identifier.citationGeophysical Research Letters, 2004; 31(10):L10103en
dc.identifier.issn0094-8276en
dc.identifier.urihttp://hdl.handle.net/2440/54958-
dc.description.abstractAlthough only a minor constituent of the earth's upper atmosphere, nitric oxide (NO) plays a major role in infrared auroral emissions due to radiation from vibrationally excited (NO*) states. The main process leading to the production of these excited molecules was thought to be chemiluminescence, whereby excited nitrogen atoms interact with oxygen molecules to form vibrationally excited nitric oxide (NO*) and atomic oxygen. Here we show evidence that a different production mechanism for NO*, due to low energy electron impact excitation of NO molecules, is responsible for more than 30% of the NO auroral emission near 5 μm.en
dc.description.statementofresponsibilityL. Campbell, M. J. Brunger, Z. Lj. Petrovic, M. Jelisavcic, R. Panajotovic and S. J. Buckmanen
dc.language.isoenen
dc.publisherAmerican Geophysical Unionen
dc.titleInfrared auroral emissions driven by resonant electron impact excitation of NO moleculesen
dc.typeJournal articleen
dc.contributor.schoolSchool of Chemistry and Physics : Physics and Mathematical Physicsen
dc.identifier.doi10.1029/2003GL019151en
Appears in Collections:Physics publications

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