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Magnetic Production of Extragalactic Jets
Published online by Cambridge University Press: 19 July 2016
Abstract
Relativistic jets are formed by plasma injected into the rapidly rotating magnetosphere of accretion disks. The accretion disk generates a dipolar or a quadrupolar magnetosphere which also immerses the black hole. We present self-consistent solutions for the structure of this magnetosphere based on the Grad-Schlüter-Shafranov equation for the poloidal magnetic flux. The resulting supermagnetosonic jets consist of a nested family of magnetic surfaces filled with normal plasma flowing along the rotational axis of the central object.
- Type
- 8. The Role of Magnetic Fields in Radio Source Jets and Extended Radio Lobes
- Information
- Symposium - International Astronomical Union , Volume 140: Galactic and Intergalactic Magnetic Fields , 1990 , pp. 413 - 417
- Copyright
- Copyright © Kluwer 1990