MHD model of astrophysical jets

Details MHD model of astrophysical jets MHD model of astrophysical jets

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000phla..276..257b&link_type=abstract

Physics Letters A, Volume 276, Issue 5-6, p. 257-266.

Physics

3

Scientific paper

Astrophysical jets are modelled by the exact axially symmetric equilibria of plasma in the gravitational field of an attracting center. The derived solutions have an arbitrary constant partition between the plasma magnetic and kinetic energy and generalize the Chandrasekhar equipartition solution. The obtained equilibria are ergodic in variable /z and depend on an arbitrary integer /N and arbitrary parameters β,a1,...,aN-1, b1,...,bN-1. Near the attracting center, the solutions have either an accretion hyperboloid or disk or cone. The latter does not depend on the above parameters and has the semi-vertical angle of 60°.

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