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| Titel |
Doppler temperatures from O(1D) airglow in the daytime thermosphere as observed by the Wind Imaging Interferometer (WINDII) on the UARS satellite |
| VerfasserIn |
C. Lathuillere, W. A. Gault, B. Lamballais, Y. J. Rochon, B. H. Solheim |
| Medientyp |
Artikel
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| Sprache |
Englisch
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| ISSN |
0992-7689
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| Digitales Dokument |
URL |
| Erschienen |
In: Annales Geophysicae ; 20, no. 2 ; Nr. 20, no. 2, S.203-212 |
| Datensatznummer |
250014356
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| Publikation (Nr.) |
 copernicus.org/angeo-20-203-2002.pdf |
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| Zusammenfassung |
From 1992 to 1997, the
WINDII interferometer on board the UARS satellite acquired a large set of
thermospheric data from the O(1D) and O(1S) airglows. We
report here for the first time on daytime O(1D) Doppler temperatures
obtained with version 5.11 of the WINDII data processing software. Using a
statistical analysis of the temperatures independently measured by the two
WINDII fields of view, we estimate that the temperature variations larger than
40 K can be considered as geophysical. Comparisons of WINDII temperatures
measured during magnetically quiet days with temperatures obtained by the
MSIS-90 and DTM-94 thermospheric models show a 100 K bias. We demonstrate,
however, that the modeled temperature variations represent very well the mean
temperature variation observed by WINDII over 4 years. We also show that the
observed latitudinal/local time variation is in very good agreement with the
two empirical models. Finally, the temperature variations during a magnetically
disturbed day are found to be qualitatively well represented in form by the
models, but largely underestimated. The presence of non-thermal atoms and
instrument related issues are discussed as possible explanations for the 100 K
bias between the WINDII Doppler temperatures and the empirical models.
Key words. Atmospheric composition
and structure (air-glow and aurora; pressure, density and temperature;
instruments and techniques) |
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