Abstract A brief report is given on the characteristics of solar flares from the active region Boulder 2372. It is interesting to note the morphological similarity (homology) between many of these events, most likely caused by the overall constancy of the magnetic field configuration. Under closer examination this first-order homology breaks down, a fact that may help us understand the basis of the flare mechanism.
The flares of April, 1980
Advances in Space Research ; 2 , 11 ; 101-104
01.01.1983
4 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
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