naa a22 4500 510790313 CHVBK 20180411083317.0 cr unu---uuuuu 180411e20130401xx s 000 0 eng 10.1134/S1063773713040014 doi (NATIONALLICENCE)springer-10.1134/S1063773713040014 On the structure of the magnetic field near a black hole in active galactic nuclei [Elektronische Daten] [V. Beskin, A. Zheltoukhov] 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 ΩF near the rotation axis of the black hole can be smaller than ΩH/2. This result is consistent with the latest numerical simulations. Pleiades Publishing, Ltd., 2013 magnetohydrodynamics nationallicence black holes nationallicence Beskin V. Lebedev Physical Institute, Russian Academy of Sciences, Leninskii pr. 53, 119991, Moscow, Russia aut Zheltoukhov A. Lebedev Physical Institute, Russian Academy of Sciences, Leninskii pr. 53, 119991, Moscow, Russia aut Astronomy Letters SP MAIK Nauka/Interperiodica 39/4(2013-04-01), 215-220 1063-7737 39:4<215 2013 39 11443 https://doi.org/10.1134/S1063773713040014 text/html Onlinezugriff via DOI 1 research-article jats NATIONALLICENCE 856 40 https://doi.org/10.1134/S1063773713040014 text/html Onlinezugriff via DOI NATIONALLICENCE 700 1- Beskin V. Lebedev Physical Institute, Russian Academy of Sciences, Leninskii pr. 53, 119991, Moscow, Russia aut NATIONALLICENCE 700 1- Zheltoukhov A. Lebedev Physical Institute, Russian Academy of Sciences, Leninskii pr. 53, 119991, Moscow, Russia aut NATIONALLICENCE 773 0- Astronomy Letters SP MAIK Nauka/Interperiodica 39/4(2013-04-01), 215-220 1063-7737 39:4<215 2013 39 11443 Metadata rights reserved Springer special CC-BY-NC licence nationallicence BK010053 XK010053 XK010000 NATIONALLICENCE NATIONALLICENCE NL-springer