On the structure of the magnetic field near a black hole in active galactic nuclei

被引：17

作者：

Beskin, V. S. ^{[1
]}

Zheltoukhov, A. A. ^{[1
]}

机构：

[1] Russian Acad Sci, PN Lebedev Phys Inst, Moscow 119991, Russia

来源：

ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 2013年 / 39卷 / 04期

关键词：

magnetohydrodynamics; black holes; ELECTROMAGNETIC EXTRACTION; ENERGY;

D O I：

10.1134/S1063773713040014

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Using the Grad-Shafranov equation, we consider a new analytical model of the black hole magnetosphere based on the assumption that the magnetic field is radial near the horizon and uniform (cylindrical) in the jet region. Within this model, we have managed to show that the angular velocity of particles Omega(F) near the rotation axis of the black hole can be smaller than Omega(H)/2. This result is consistent with the latest numerical simulations.

引用

页码：215 / 220

页数：6

共 15 条

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