Abstract A numerical ray tracing technique is used to study the time evolution of VLF radiation (2–3 kHz Voyager band) trapped in the heliosphere. Simulations include effects of co-rotating and merging interaction regions, heliolatitudinal dependence of solar wind speed and absorption by free-free transitions. The results imply constraints on solar wind dynamics as well as on the size and the tail geometry of the heliosphere.


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    Titel :

    Trapped VLF radiation as a signature of the dynamical processes in the heliosphere


    Beteiligte:
    Czechowski, A. (Autor:in) / Grzedzielski, S. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 13 , 6 ; 223-226


    Erscheinungsdatum :

    01.01.1993


    Format / Umfang :

    4 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch




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