Abstract The structure of the inner corona are the main sources of the XUV line radiation from the sun. The line intensities are determined by the temperature and density of the plasma via the differential emission measure (DEM) distribution. The DEM contains a lot of information concerning the physics of the coronal features; the methods to evaluate differential emission measure distribution from the observational data are reviewed and discussed.


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    Titel :

    Models for inner corona parameters


    Beteiligte:

    Erschienen in:

    Advances in Space Research ; 11 , 1 ; 281-292


    Erscheinungsdatum :

    01.01.1991


    Format / Umfang :

    12 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch



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