Speakers
Dr
Miljenko Cemeljic
(NCAC, Poland & ASIAA, Taiwan)Prof.
Feng Yuan
(Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China)Mr
Hai Yang
(Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China)
Description
In our 3D numerical simulations of accretion disk around a supermassive black hole with the GRMHD code Athena++, we follow the time evolution of magnetic field. In the case of SANE configuration, with multiple loops of oppositely directed initial poloidal magnetic field in the torus around a black hole, we follow the forming of flux ropes atop the disk, and their release into corona.
Primary author
Dr
Miljenko Cemeljic
(NCAC, Poland & ASIAA, Taiwan)