AbstractA large number of coronal heating theories have been proposed and most of them can be labeled as AC or DC heating theories. Here a short description of these two main theories is given, and the results of a DC heating model simulation is explained in more detail. As a result of that model, arguments are given for putting emphasis on launching a very fast spectrograph, ideally a imaging spectrograph as soon as possible.


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    Titel :

    Coronal dynamics and heating theories


    Beteiligte:

    Erschienen in:

    Advances in Space Research ; 43 , 1 ; 108-112


    Erscheinungsdatum :

    2008-05-24


    Format / Umfang :

    5 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch




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