Some Properties of an Axisymmetric Pulsar Magnetosphere Constructed by Numerical Calculation
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概要
- 論文の詳細を見る
We have explored the magnetosphere described by a numerical solution for an Axisymmetric rotating field satisfying the force free and ideal MHD conditions everywhere. The electric current distribution is determined by the requirement of continuity and smoothness of the flux function across the light cylinder. The overall magnetic field structure is obtained using the numerical result. We also checked the drift velocity of a charged particle, which is caused by the resultant electric and magnetic fields. It is found that the velocity exceeds the light speed beyond a few times the size of the light cylinder. This fact suggests the breakdown of some underlying assumptions.
- 理論物理学刊行会の論文
- 2003-04-25
著者
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Ogura J
Department Of Physics Hiroshima University
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Ogura Jun
Department Of Physics Faculty Of Sciences Saitama University
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Ogura Jun
Department Of Neurology Kohnan Hospital
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Kojima Yasuaki
Graduate School Of Engineering Hiroshima University
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KOJIMA Yasufumi
Department of Physics, Tokyo Metropolitan University
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Kojima Y
Department Of Physics Hiroshima University
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Kojima Yasufumi
Department Of Physics Hiroshima University
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Kashiv Y.
Advanced Science Research Center Japan Atomic Energy Agency
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KOJIMA Yasufumi
Department of Physics, University of Wales
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