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.


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    Title :

    The flares of April, 1980


    Contributors:

    Published in:

    Advances in Space Research ; 2 , 11 ; 101-104


    Publication date :

    1983-01-01


    Size :

    4 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English



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