AbstractThe long-term variations in solar activity are studied using the dataset comprised of sunspot number and 14 C radioisotope timeseries. We use a novel S 200 index to identify possible past Grand Minima (GM). The Maunder, Oort, Wolf and Spörer Minima fall in phase with the minimum of S 200 index. We also show GM develop in clusters, with a separation of about 400–600years between individual GM. Extending these found similarities to modern solar activity, it is predicted that next grand solar minimum may occur in about 2090 ± 20 .


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    Titel :

    On the timing of the next great solar activity minimum


    Beteiligte:
    Tlatov, A.G. (Autor:in) / Pevtsov, A.A. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 60 , 5 ; 1108-1114


    Erscheinungsdatum :

    2017-05-09


    Format / Umfang :

    7 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch




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