The principles of constructing the model are considered in this paper, together with the issues of its components and physical algorithm. The main emphasis is placed on the cause-and-effect relationships between the structure and dynamics of the solar and interplanetary media and the motion of solar cosmic ray particles. The specific features of the initial phase of motion of the particles after their acceleration in a solar flare are considered, as well as the subsequent phase of further particle propagation in the solar corona, and the phase of motion in the heliosphere. The processes of transport of charged particles in flare plasma ejections are considered in detail.


    Zugriff

    Zugriff prüfen

    Verfügbarkeit in meiner Bibliothek prüfen

    Bestellung bei Subito €


    Exportieren, teilen und zitieren



    Titel :

    The reflection model for propagation of solar cosmic rays


    Weitere Titelangaben:

    Cosmic Res


    Beteiligte:

    Erschienen in:

    Cosmic Research ; 45 , 1 ; 9-15


    Erscheinungsdatum :

    2007-02-01


    Format / Umfang :

    7 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch




    The reflection model for propagation of solar cosmic rays

    Lyubimov, G. P. / Grigorenko, E. E. | Online Contents | 2007


    Propagation of Solar Cosmic Rays in the Solar Wind

    Mclntosh, Patrick S. / Dryer, Murray | AIAA | 1972


    Propagation and origin of ultra high-energy cosmic rays

    Berezinsky, Veniamin | Elsevier | 2007


    Propagation and origin of ultra high-energy cosmic rays

    Berezinsky, Veniamin | Online Contents | 2008


    Propagation and origin of ultra high-energy cosmic rays

    Berezinsky, Veniamin | Online Contents | 2008