AbstractThis contribution is mostly about phenomenology of what we see in space–time evolution of coronal green line brightness (CGLB), including its cyclic variations. Our own database (1943–2001) of the coronal Fe XIV 530.3nm emission line intensities is used to display different aspects of the large-scale CGLB regularities and cyclic behaviour. Hemispheric asymmetry and relation of the longitudinal CGLB distribution to the rotational characteristics of the solar corona are particularly underlined.


    Zugriff

    Zugriff prüfen

    Verfügbarkeit in meiner Bibliothek prüfen

    Bestellung bei Subito €


    Exportieren, teilen und zitieren



    Titel :

    Coronal manifestations of solar variability


    Beteiligte:
    Sýkora, J. (Autor:in) / Rybák, J. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 35 , 3 ; 393-399


    Erscheinungsdatum :

    2005-03-09


    Format / Umfang :

    7 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch




    Coronal manifestations of solar variability

    Sy@4kora, J. | Online Contents | 2005


    Coronal manifestations of solar variability

    Sýkora, J. / Rybák, J. / International Council of Scientific Unions | British Library Conference Proceedings | 2005


    Variability of the Solar Coronal Rotation

    Vats, H.Om | Online Contents | 1999


    Variability of the Solar Coronal Rotation

    Om Vats, H. / Deshpande, M. R. / Mehta, M. et al. | British Library Conference Proceedings | 1999


    Coronal Manifestations of Oscillations: A Numerical Model

    Andreev, A. S. / Kosovichev, A. G. | British Library Online Contents | 1995