Abstract We compared fluxes of the 1–100 MeV solar energetic particles (SEP) measured in the interplanetary medium (ACE) and in the magnetosphere (Universitetsky-Tatiana, POES—in polar caps, and GOES-11—at geosynchronous orbit) during several SEP events of 2005–2006. Peak intensities of the SEP fluxes inside and outside the magnetosphere were compared for each event. It is shown that observed inside-outside difference depends mainly on direction of interplanetary magnetic field (IMF), on degree of the SEP anisotropy (pitch-angle distribution) in IMF, and on distance of the dayside magnetopause from the Earth.


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    Titel :

    Some features of solar cosmic ray penetration into the Earth’s magnetosphere


    Beteiligte:
    Vlasova, N. A. (Autor:in) / Pavlov, N. N. (Autor:in) / Panasyuk, M. I. (Autor:in) / Vedenkin, N. N. (Autor:in) / Ivanova, T. A. (Autor:in) / Lyubimov, G. P. (Autor:in) / Reizman, S. Ya. (Autor:in) / Tulupov, V. I. (Autor:in)

    Erschienen in:

    Cosmic Research ; 49 , 6 ; 485-499


    Erscheinungsdatum :

    26.11.2011


    Format / Umfang :

    15 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch




    Some features of solar cosmic ray penetration into the Earth’s magnetosphere

    Vlasova, N. A. / Pavlov, N. N. / Panasyuk, M. I. et al. | Online Contents | 2011



    Penetration of solar cosmic rays into the Earth’s magnetosphere on January 28, 2012

    Vlasova, N. A. / Ginzburg, E. A. / Kalegaev, V. V. et al. | Springer Verlag | 2013


    Penetration of solar cosmic rays into the Earth’s magnetosphere on January 28, 2012

    Vlasova, N. A. / Ginzburg, E. A. / Kalegaev, V. V. et al. | Online Contents | 2013