Observations of the temporal evolution of loop BC in soft X-rays in the November 5, 1980 flare are reviewed. Calculations are performed to model this evolution. The most consistent interpretation involving a minimum amount of energy is the following: thermal heating near B gives rise to a conduction front which moves out along the loop uninhibited for about 27 s, and beam heating near C gives rise to a second conduction front which moves in the opposite direction and prevents any energy reaching C by thermal conduction from B.


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    Titel :

    The relative contribution of beam versus thermally produced X-rays in the large loop of the 5 November 1980 flare


    Beteiligte:
    Smith, D. F. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    1986-01-01



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


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