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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
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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
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