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13 December 2018 Modeling atomic oxygen nightglow during the strong magnetic storm on 20 November 2003
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Proceedings Volume 10833, 24th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics; 108339R (2018) https://doi.org/10.1117/12.2504352
Event: XXIV International Symposium, Atmospheric and Ocean Optics, Atmospheric Physics, 2018, Tomsk, Russian Federation
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).
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
A. V. Tashchilin and L. A. Leonovich "Modeling atomic oxygen nightglow during the strong magnetic storm on 20 November 2003", Proc. SPIE 10833, 24th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics, 108339R (13 December 2018); https://doi.org/10.1117/12.2504352
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