Abstract H-alpha observations of flares of importance S are used for determining the scales of preflare activations as well as in studying the spatial location of the flares relative to chromospheric structures. The results obtained indicate that there is a close relationship of solar flares with supergranulation structure of active regions.
The manifestation of supergranulation structures of active regions during solar flares
Advances in Space Research ; 8 , 11 ; 141-144
1989-01-01
4 pages
Article (Journal)
Electronic Resource
English
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