Abstract Low frequency magnetic field turbulence is described in terms of an ideal gas of circularly polarized Alfvén solitons. This approach leads to a magnetic field power spectrum with a broad local maximum and an exponential decay and is able to reproduce a special power spectrum obtained by the AMPTE/IRM spacecraft mission upstream of Earth's bow shock.


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    Titel :

    On low frequency magnetic field turbulence upstream of earth's bow shock


    Beteiligte:
    Mann, G. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 11 , 9 ; 249-252


    Erscheinungsdatum :

    01.01.1991


    Format / Umfang :

    4 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch




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