Generation of shear Alfvén waves by a rotating magnetic field source: Three-dimensional simulations

2011 ◽  
Vol 18 (3) ◽  
pp. 032113 ◽  
Author(s):  
A. V. Karavaev ◽  
N. A. Gumerov ◽  
K. Papadopoulos ◽  
Xi Shao ◽  
A. S. Sharma ◽  
...  
2009 ◽  
Vol 16 (9) ◽  
pp. 092106 ◽  
Author(s):  
A. Gigliotti ◽  
W. Gekelman ◽  
P. Pribyl ◽  
S. Vincena ◽  
A. Karavaev ◽  
...  

1981 ◽  
Vol 46 (26) ◽  
pp. 1675-1678 ◽  
Author(s):  
W. W. Lee ◽  
M. S. Chance ◽  
H. Okuda

2018 ◽  
Vol 27 (10) ◽  
pp. 1844006
Author(s):  
A. Dorodnitsyn ◽  
T. Kallman

Large scale magnetic field can be easily dragged from galactic scales toward AGN along with accreting gas. There, it can contribute to both the formation of AGN “torus” and help to remove angular momentum from the gas which fuels AGN accretion disk. However the dynamics of such gas is also strongly influenced by the radiative feedback from the inner accretion disk. Here we present results from the three-dimensional simulations of pc-scale accretion which is exposed to intense X-ray heating.


2011 ◽  
Vol 53 (2) ◽  
pp. 025009 ◽  
Author(s):  
Alessandro Biancalani ◽  
Liu Chen ◽  
Francesco Pegoraro ◽  
Fulvio Zonca

1985 ◽  
Vol 161 (1) ◽  
pp. 21-47 ◽  
Author(s):  
C.Z Cheng ◽  
Liu Chen ◽  
M.S Chance

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