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9.15. Theoretical method for treating force-free black hole magnetosphere in non-stationary and non-axisymmetric state

Published online by Cambridge University Press:  25 May 2016

T. Uchida
T. Uchida*
Affiliation:
Division of Theoretical Astrophysics, National Astronomical Observatory, Mitaka, Tokyo 181, Japan

Extract

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The force-free approximation is a very useful method in studies of the global electromagnetic structure of the magnetospheres around the relativistic astronomical bodies. However, its application has almost been restricted to the stationary and axisymmetric configuration. In this work, we remove this restriction and construct a general method for treating the force-free electromagnetic field.

Type
Part III. Black Holes and Central Activity
Information
Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 411 - 412
Copyright
Copyright © Kluwer 1998