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Modeling atomic oxygen nightglow during the strong magnetic storm on 20 November 2003
Author(s): A. V. Tashchilin; L. A. Leonovich
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Paper Abstract

Intensity variations in red line of atomic oxygen emission were analyzed using the ionosphere-plasmasphere coupling model. These variations were caused by precipitation of energetic electrons from the magnetosphere during the 20 November 2003 geomagnetic storm. The findings were compared to the optical data measured in Geophysical observatory of the ISTP SB RAS (520 N, 1030 E).

Paper Details

Date Published: 13 December 2018
PDF: 4 pages
Proc. SPIE 10833, 24th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics, 108339R (13 December 2018); doi: 10.1117/12.2504352
Show Author Affiliations
A. V. Tashchilin, Institute of Solar-Terrestrial Physics of the SB RAS (Russian Federation)
L. A. Leonovich, Institute of Solar-Terrestrial Physics of the SB RAS (Russian Federation)


Published in SPIE Proceedings Vol. 10833:
24th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics
Gennadii G. Matvienko; Oleg A. Romanovskii, Editor(s)

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