Aurora dynamics in the far ultraviolet during the magnetic storm of March 2-3, 1982

Details Aurora dynamics in the far ultraviolet during the magnetic storm of March 2-3, 1982 Aurora dynamics in the far ultraviolet during the magnetic storm of March 2-3, 1982

Jul 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987kosis..25..566b&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 25, July-Aug. 1987, p. 566-576. In Russian.

Physics

Auroras, Magnetic Storms, Spectrophotometry, Ultraviolet Radiation, Charged Particles, Earth Magnetosphere, Hydrogen Atoms, Intercosmos Satellites, Night, Oxygen Atoms, Particle Precipitation

Scientific paper

Research on auroras in the ultraviolet is reviewed, and spectrophotometric data obtained at H I 1216 A, O I 1304 A, O I 1356 A, and gamma (1,1) NO 2246 A on the Intercosmos-Bulgaria-1300 satellite are examined. Particular attention is given to the development of the magnetic storm of March 2-3, 1982. Consideration is given to the role of charged particles precipitating from the nocturnal magnetosphere as an additional source of the excitation of the observed glow from atomic hydrogen and oxygen as well as of the gamma (1,1) band of NO.

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