A brief overview of the physics thought to determine the properties of the heliospheric termination shock is given and the central role of hot interstellar pick-up ions and cosmic rays is emphasized.


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    Title :

    The termination shock: Physical processes


    Contributors:
    Zank, G. P. (author) / Cairns, I. H. (author) / Webb, G. M. (author)

    Published in:

    Publication date :

    1995-01-01



    Type of media :

    Miscellaneous


    Type of material :

    No indication


    Language :

    English


    Keywords :


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