Abstract 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.


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    Title :

    The reflection model for propagation of solar cosmic rays


    Contributors:

    Published in:

    Publication date :

    2007




    Type of media :

    Article (Journal)


    Type of material :

    Print


    Language :

    English



    Classification :

    BKL:    50.93 Weltraumforschung / 39.00 Astronomie: Allgemeines / 55.60 Raumfahrttechnik
    Local classification TIB:    770/3520/8000



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    Composition of Solar cosmic rays

    Fichtel, C. E. | NTRS | 1962


    Composition of Solar Cosmic Rays

    S. Biswas / C. E. Fichtel | NTIS | 1965


    Cosmic rays

    Vernov, S. N. ;Dorman, L. I. | TIBKAT | 1964