Plasma flow in the magnetosphere of an axisymmetric rotator

Details Plasma flow in the magnetosphere of an axisymmetric rotator Plasma flow in the magnetosphere of an axisymmetric rotator

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996mnras.280...39b&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 280, Issue 1, pp. 39-52.

Astronomy and Astrophysics

Astronomy

19

Mhd, Solar Wind, Stars: Magnetic Fields, Stars: Mass-Loss, Pulsars: General, Stars: Rotation

Scientific paper

To obtain the solution of the problem of a stationary plasma ejection by a magnetized rotating star the 3D non-stationary axially symmetric problem is solved numerically. The solution for a cold non-relativistic plasma ejected by a star having a monopole-like magnetic field is obtained. A search for discontinuities in the solution is performed. It is shown that in the non-relativistic case almost 50 per cent of the Poynting flux can be transformed into the kinetic energy of the plasma. The problem of the stability of the flow is discussed.

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