AbstractExisting coronagraphic measurements, obtained by the world-wide net of observatories, are used to characterize the large-scale variabilities and periodicities in the 530.3 nm emission corona over the period 1943–1991. Specifically, the time-latitude distribution of the coronal brightness is shown and in this connection the double maxima of the solar cycles, fine structure of the butterfly diagrams, N-S asymmetry and two modes - rigid and differential - of the coronal rotation are discussed.


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    Titel :

    The large-scale behaviour of the green emission corona FeXIV 530.3 NM over the last 4.5 solar activity cycles


    Beteiligte:
    Sykora, J. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    1993-01-01


    Format / Umfang :

    4 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch





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