Abstract Measurements of the general magnetic field of the Sun seen as a star were performed over last 45years by the CrAO and five other observatories (1968–2012, nearly 23 thousand daily strengths B). Analysis of the B time series showed that the most substantial long-term period of the field variation is the Hale’s cycle 22years, which cannot be explained by dynamo theory. It reveals a saw-edged profile, indicating perhaps a cosmic origin of the cycle.


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    Titel :

    On the origin of the 22years solar cycle


    Beteiligte:
    Kotov, V.A. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 55 , 3 ; 979-981


    Erscheinungsdatum :

    2014-12-04


    Format / Umfang :

    3 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch




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