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.


    Zugriff

    Zugriff über TIB

    Verfügbarkeit in meiner Bibliothek prüfen

    Bestellung bei Subito €


    Exportieren, teilen und zitieren



    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:

    Erscheinungsdatum :

    2009




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Print


    Sprache :

    Englisch


    Schlagwörter :

    Klassifikation :

    BKL:    55.60 Raumfahrttechnik / 39.00 Astronomie: Allgemeines / 50.93 Weltraumforschung
    Lokalklassifikation TIB:    770/3520/8000



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

    Kaplan, L. G. / Otkidychev, P. A. | Springer Verlag | 2009


    Vortex generating apparatus and vortex generating method

    TANAKA MOTOFUMI / OSAKO TOSHIKI / SHIODA KAZUNORI et al. | Europäisches Patentamt | 2018

    Freier Zugriff

    Magnetic field reconnection in solar and stellar flares

    Kundu, M.R. / White, S.M. | Elsevier | 1990


    Magnetic-field generating circuit

    KUROKAWA TAKASHI | Europäisches Patentamt | 2022

    Freier Zugriff

    SHIP INCLUDING VORTEX GENERATING FINS

    LEE SWUNG HO | Europäisches Patentamt | 2018

    Freier Zugriff