Abstract On the basis of an analysis of the data of multi-satellite observations of magnetic clouds at the path Venus-Earth, the dependence of their geoeffectiveness on the orientation in the ecliptic plane and position relative to the Sun-Earth line is determined in the paper. The cloud parameters were determined on the basis of the model of a force-free cylindrical flux rope. The search for magnetic clouds in the flow of data from the monitoring space vehicle was performed using a special-purpose computer program.


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    Titel :

    Manifestation of configurations of magnetic clouds of the solar wind in geomagnetic activity


    Beteiligte:
    Barkhatov, N. A. (Autor:in) / Kalinina, E. A. (Autor:in) / Levitin, A. E. (Autor:in)

    Erschienen in:

    Cosmic Research ; 47 , 4 ; 268-278


    Erscheinungsdatum :

    2009-08-01


    Format / Umfang :

    11 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch




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