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

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

Jun 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cosre..47..217k&link_type=abstract

Cosmic Research, Volume 47, Issue 3, pp.217-225

Physics

98.58.Ay

Scientific paper

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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