AbstractThe 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.


    Zugriff

    Zugriff prüfen

    Verfügbarkeit in meiner Bibliothek prüfen

    Bestellung bei Subito €


    Exportieren, teilen und zitieren



    Titel :

    The physics of coronal closed-filed structures


    Beteiligte:

    Erschienen in:

    Advances in Space Research ; 14 , 4 ; 139-148


    Erscheinungsdatum :

    01.01.1993


    Format / Umfang :

    10 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch



    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-field structures

    Antiochos, Spiro K. | NTRS | 1994


    Coronal structures

    Curtis, G. W. / Dunn, R. B. / Orrall, F. Q. | NTRS | 1965


    Coronal physics from eclipse observations

    Koutchmy, S. | Elsevier | 1993