Computer Science
Scientific paper
Oct 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ge%26ae..32...57s&link_type=abstract
Geomagnetizm i Aehronomiya (ISSN 0016-7940), vol. 32, no. 5, p. 57-61.
Computer Science
Auroral Zones, Geomagnetism, Interplanetary Magnetic Fields, Ionospheric Disturbances, Magnetic Storms, Magnetosphere-Ionosphere Coupling, Solar Wind
Scientific paper
It is pointed out that the determination of indexes characterizing the intensity of auroral electrojets with respect to horizontal components during magnetic storms requires data from subauroral observatories. As the initial intensity of a magnetic disturbance increases, so does its susceptibility to solar-wind parameters. The higher the level of the disturbance, the more intense is the western electrojet.
Fel'Dshtejn Ya. I.
Sumaruk P. V.
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