Abstract Conditions for confining the heliosphere to a relatively small size of 55(75) AU are discussed. It is suggested that the required additional pressure of 1–2 eV cm−3 (over LISM pressure at infinity) can be provided by a cloud of suprathermal particles (including ACR) trapped within a turbulent stagnating region ahead of the heliosphere and containing a large fraction of the original solar wind energy.


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    Titel :

    Confinement of the heliosphere and relevant physical processes


    Beteiligte:

    Erschienen in:

    Erscheinungsdatum :

    01.01.1989


    Format / Umfang :

    4 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch



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