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A method of predictions geomagnetic activity based on a coronal model of relations between solar and geomagnetic activities (1979)

Halenka, J.

In: CASI

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Publication Date: 2006-01-16

Description: A method developed to predict both disturbed and quiet geomagnetic periods is described. The method uses solar situations along the CM with the key role of filaments, giving indirect evidence of types of directly unobservable coronal structures above them. The time lag, not to be interpreted in terms of propagation speed, between the CM activity and the commencement of the geomagnetic response is about one to two days. Solar phenomena serve as indicators within approximately 10 deg of the CM and up to the zone of high latitude filaments.

Keywords: GEOPHYSICS

Type: NOAA Solar-Terrest. Predictions Proc., Vol. 1; p 44-60

Format: text

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