Physics
Scientific paper
Jul 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992crlj...39..233t&link_type=abstract
Communications Research Laboratory, Journal (ISSN 0914-9260), vol. 39, no. 2, p. 233-247.
Physics
Coronal Holes, Ionospheric Disturbances, Magnetic Storms, Solar Activity Effects, Solar Flares, Solar Prominences, Interplanetary Medium, Solar Radio Bursts, Solar Terrestrial Interactions, Solar X-Rays
Scientific paper
In order to determine the origin of the geomagnetic storm of Nov. 30, 1988, solar weather is analyzed with respect to the following three phenomena: flare activity, high-speed corotating regions or coronal holes, and filament disappearances. The results of the analysis indicate that the possibility that the geomagnetic disturbance was caused by a solar flare activity is minimal. Strong evidence is found for the effect of a corotating high-speed region on the geomagnetic field. The effect of filament disappearance is believed to be the most probable factor.
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