Titlebook: Black Hole Gravitohydromagnetics; Brian Punsly Book 20011st edition Springer-Verlag Berlin Heidelberg 2001 Activie Galactic Nuclei.Black H

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Perfect MHD Winds and Waves in the Ergosphere,t horizon is an asymptotic infinity to MHD winds and waves similar to the infinity of the semi-infinite plasma filled waveguide of Sect. 2.9.4. As we found in the study of electrodynamics of black holes in Chap. 4, the spacetime near the event horizon has no significance for the determination of a g

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Ergospheric Disk Dynamos,e GHM interaction of flux tubes that thread the equatorial plane of the ergosphere and therefore not the horizon. In this chapter we look at a highly idealized model in which a disk of ergospheric plasma is the dynamo (see Fig. 8.1). This has two simplifying features. Firstly, the equatorial disk ac

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Book 20011st editioneractions that combine the effects of gravity and a strong magnetic field, in the vicinity (ergosphere) of a rapidly rotating black hole. This topic was created in response to the astrophysical quest to understand the central engines of radio loud extragalactic radio sources. The theory describes a

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Relativistic Plasma Physics,an induce currents to flow in a wind far from the hole if, and only if, a wave packet carrying the appropriate information requiring the current flow is transmitted from the ergospheric plasma and received by the wind plasma far from the hole. The relativistic structure of plasma waves is the prime emphasis of this chapter.

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