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Wind Acceleration in Pulsar Magnetospheres

Published online by Cambridge University Press:  12 April 2016

Masaaki Takahashi  and
Shinpei Shibata
Masaaki Takahashi
Affiliation:
Department of Physics and Astronomy, Aichi University of Education Hirosawa, Igaya-cho, Kariya 448, Japan
Shinpei Shibata
Affiliation:
Department of Physics, Yamagata UniversityYamagata 990, Japan

Abstract

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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

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