AbstractTwo phenomena connected with the maximum phase of the 11-year solar cycle in the galactic cosmic ray intensity – the change in the energy dependence of the intensity variations and the double-peak structure in the intensity modulation time profile – are considered for the last five solar cycles (Nos. 19–23). The distinct 22-year cycle in the magnitude of the so called energy hysteresis is observed.The periods of the solar cycle maximum phase in the galactic cosmic ray intensity, characterized by the specific energy dependence of the intensity, are estimated. It is found that the double-peak structures belonging to the solar cycle maximum phase and those around it are very similar both in the amplitude and in its energy dependence.


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    Titel :

    The structure of the solar cycle maximum phase in the galactic cosmic ray 11-year variation


    Beteiligte:

    Erschienen in:

    Advances in Space Research ; 35 , 12 ; 2124-2128


    Erscheinungsdatum :

    2004-11-05


    Format / Umfang :

    5 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch





    The structure of the solar cycle maximum phase in the galactic cosmic ray 11-year variation

    Krainev, M. B. / Bazilevskaya, G. A. / International Council of Scientific Unions | British Library Conference Proceedings | 2005


    Prediction of Galactic Cosmic Ray Modulation by CME at Solar Cycle 23 Maximum

    Ahluwalia, H. S. / International Council of Scientific Unions | British Library Conference Proceedings | 2000