The properties of closed coronal loops are reviewed. First we discuss the main features of the static, hot loop models. In these models thermal conduction plays the dominant role in determining the temperature and density structure. Next the cool loop models and their implications for solar observations are discussed. Finally, some new theoretical results on coronal abundances are presented. It is argued that chromospheric evaporation, which is a basic feature of the hot models, can account for the observed anomalies in the coronal element abundances.


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    Titel :

    The physics of coronal closed-field structures


    Beteiligte:

    Erschienen in:

    Erscheinungsdatum :

    1994-04-01



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    The Physics of Coronal Closed-Field Structures

    Antiochos, Spiro K. | Online Contents | 1994


    The Physics of Coronal Closed-Field Structures

    Antiochos, S. K. / COSPAR | British Library Conference Proceedings | 1994


    The physics of coronal closed-filed structures

    Antiochos, Spiro K. | Elsevier | 1993


    Coronal Physics from Eclipse Observations

    Koutchmy, S. | Online Contents | 1994


    Coronal Physics from Eclipse Observations

    Koutchmy, S. / COSPAR | British Library Conference Proceedings | 1994