Ionospheric disturbances during November 30-December 1, 1988. II - Solar weather related to the earth disturbances during the event

Physics

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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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