Asymptotic structure of magnetically driven MHD wind

Details Asymptotic structure of magnetically driven MHD wind Asymptotic structure of magnetically driven MHD wind

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ppcn.conf..321n&link_type=abstract

In ESA, Fourth International Toki Conference on Plasma Physics and Controlled Nuclear Fusion p 321-323 (SEE N94-22624 05-75)

Physics

Plasma Physics

Magnetic Field Configurations, Relativistic Plasmas, Self Consistent Fields, Stellar Winds, Asymptotic Properties, Magnetohydrodynamic Flow, Plasma Density, Plasma Jets, Poloidal Flux

Scientific paper

The asymptotic structure of plasma wind is discussed. By solving the special relativistic magnetohydrodynamic (MHD) equations for transfield force balance, an analytic self consistent solution is obtained for the steady and axisymmetric magnetically driven wind in the limit of viscousless, pressureless and resistiveless plasmas. In this solution, all the field lines are asymptotically conical. The inclination angle of each field line from the equatorial plane is determined. The thin jet solution as in radio loud active galactic nuclei or the equatorial wind solution can be obtained.

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