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Remote determination of auroral energy characteristics during substorm activity
Center for Space Sciences, University of Texas at Dallas, Richardson, TX.
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1997 (English)In: Geophysical Research Letters, ISSN 0094-8276, E-ISSN 1944-8007, Vol. 24, 995-998 p.Article in journal (Refereed) Published
Abstract [en]

Ultraviolet auroral images from the Ultraviolet Imager (UVI) onboard the POLAR satellite can be used as quantitative remote diagnostics of the auroral regions, yielding estimates of incident energy characteristics, compositional changes, and other higher order data products. Here incident energy estimates derived from UVI are compared with in situ measurements of the same parameters from an overflight by the DMSP F12 satellite coincident with the UVI image times during substorm activity occurring on May 19, 1996. This event was simultaneously observed by WIND, GEOTAIL, INTERBALL, DMSP and NOAA spacecraft as well as by POLAR.

Place, publisher, year, edition, pages
1997. Vol. 24, 995-998 p.
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Fusion, Plasma and Space Physics
Identifiers
URN: urn:nbn:se:kth:diva-93360DOI: 10.1029/97GL00864OAI: oai:DiVA.org:kth-93360DiVA: diva2:515736
Note
NR 20140805Available from: 2012-04-15 Created: 2012-04-15 Last updated: 2017-12-07Bibliographically approved

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