Abstract The difference in viscous properties of proton and electron gases in fully ionized hydrogen plasma is shown to result in a possibility of generation in this plasma of the magnetic field, even if initially there was no field. As an example, a simplified planar stationary model of a magnetohydrodynamic process of the eddy sink type is considered. It is demonstrated that the intensity of the generated magnetic field strongly depends on plasma temperature, so that the range T = 100000–500000 K corresponds to the range of maximum magnetic induction B = 50–2700 G. Such values are frequently observed in ordinary stars, in particular, in solar flares.


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    Titel :

    A mechanism for generating magnetic field by vortex processes in stellar plasma


    Beteiligte:
    Kaplan, L. G. (Autor:in) / Otkidychev, P. A. (Autor:in)

    Erschienen in:

    Cosmic Research ; 47 , 3 ; 217-225


    Erscheinungsdatum :

    2009-06-01


    Format / Umfang :

    9 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch




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