The method of characteristics has been used to solve numerically the equations of steady special relativistic MHD flows. The authors show some preliminary results which investigate the effects of a dynamically important toroidal magnetic field on the propagation of weak pressure discontinuities.
Steady, Relativistic Magnetized Jet
PANTANO, ORNELLA
1992
Abstract
The method of characteristics has been used to solve numerically the equations of steady special relativistic MHD flows. The authors show some preliminary results which investigate the effects of a dynamically important toroidal magnetic field on the propagation of weak pressure discontinuities.
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