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The response of thermospheric nitric oxide to an auroral storm. II - Auroral latitudesNOAA 6 and 7 particle measurements are used, in conjunction with a statistical model of the auroral particle precipitation, to study the response of auroral NO to the auroral storm of September 19, 1984. The results of a time-dependent photochemical calculation show that particle precipitation can more effectively produce NO than can Joule heating, in contrast to nonauroral latitudes where heating is important. Both the model and the NO data show NO increases as a result of the storm; however, the absolute magnitude of the NO in the model, as well as the amplitude of the increase, significantly exceeded what was observed. Two possible explanations for the this discrepancy are proposed.
Document ID
19900033674
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Siskind, D. E.
(Colorado Univ. Boulder, CO, United States)
Barth, C. A.
(Colorado, University Boulder, United States)
Evans, D. S.
(NOAA, Space Environment Laboratory, Boulder CO, United States)
Roble, R. G.
(High Altitude Observatory Boulder, CO, United States)
Date Acquired
August 14, 2013
Publication Date
December 1, 1989
Publication Information
Publication: Journal of Geophysical Research
Volume: 94
ISSN: 0148-0227
Subject Category
Geophysics
Accession Number
90A20729
Funding Number(s)
CONTRACT_GRANT: NASW-4091
CONTRACT_GRANT: NASA ORDER W-16320
Distribution Limits
Public
Copyright
Other

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