Hybrid simulation of shock formation for super-Alfvénic expansion of laser ablated debris through an ambient, magnetized plasma

2013 ◽  
Vol 20 (8) ◽  
pp. 082129 ◽  
Author(s):  
S. E. Clark ◽  
D. Winske ◽  
D. B. Schaeffer ◽  
E. T. Everson ◽  
A. S. Bondarenko ◽  
...  
2006 ◽  
Vol 2 (S238) ◽  
pp. 367-368
Author(s):  
Keigo Fukumura ◽  
Masaaki Takahashi ◽  
Sachiko Tsuruta

AbstractWe study magnetohydrodynamic (MHD) standing shocks in ingoing plasmas in a black hole (BH) magnetosphere. We find that low or mid latitude (non-equatorial) standing MHD shocks are both physically possible, creating very hot and/or magnetized plasma regions close to the event horizon. We also investigate the effects of the poloidal magnetic field and the BH spin on the properties of shocks and show that both effects can quantitatively affect the MHD shock solutions. MHD shock formation can be a plausible mechanism for creating high energy radiation region above an accretion disk in AGNs.


2014 ◽  
Vol 90 (4) ◽  
Author(s):  
S. E. Clark ◽  
E. T. Everson ◽  
D. B. Schaeffer ◽  
A. S. Bondarenko ◽  
C. G. Constantin ◽  
...  

2005 ◽  
Vol 298 (1-2) ◽  
pp. 369-374 ◽  
Author(s):  
V. I. Sotnikov ◽  
H. Ruhl ◽  
R. Presura ◽  
T. Cowan ◽  
J. N. Leboeuf ◽  
...  

Author(s):  
V.I. Sotnikov ◽  
H. Ruhl ◽  
R. Presura ◽  
T. Cowan ◽  
J.N. Leboeuf ◽  
...  

2006 ◽  
Author(s):  
David D. Blackwell ◽  
David N. Walker ◽  
Sarah J. Messer ◽  
William E. Amatucci

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