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Wind Acceleration in Pulsar Magnetospheres
Published online by Cambridge University Press: 12 April 2016
Abstract
To explain the pulsar wind acceleration and the energy conversion from the electromagnetic energy to the plasma’s kinetic energy between the pulsar and the nebula’s shock, we study relativistic cold ideal MHD winds in non-radial magnetic field geometry and clarify the critical conditions of trans-fast MHD winds.
- Type
- Part 6 Winds and the ISM
- Information
- International Astronomical Union Colloquium , Volume 160: Pulsars: Problems and Progress , 1996 , pp. 425 - 428
- Copyright
- Copyright © Astronomical Society of the Pacific 1996