Study of neoclassical tearing modes based on a reduced MHD model in cylindrical geometry

2005 ◽  
Vol 45 (2) ◽  
pp. 143-149 ◽  
Author(s):  
M Sato ◽  
M Wakatani
1977 ◽  
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B. Carreras ◽  
J. A. Holmes ◽  
B. V. Waddell

1993 ◽  
Vol 141 ◽  
pp. 443-445
Author(s):  
X.H. Deng ◽  
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J.M. Chen ◽  
H.Q. Zhang ◽  
G.X. Ai

AbstractThe nonlinear evolution of tearing modes in the presence of sheared mass flow is studied in the cylindrical geometry. It is demonstrated that a sufficient large sheared mass flow can destabilize the development of resistive tearing instability. It is suggested that the coupling of sheared mass flow with shear magnetic field may be a triggering of solar flares.


2008 ◽  
Vol 50 (3) ◽  
pp. 035005
Author(s):  
E V van der Plas ◽  
H J de Blank

2020 ◽  
Vol 27 (1) ◽  
pp. 012504
Author(s):  
Z. Q. Hu ◽  
C. Ye ◽  
L. Wei ◽  
Z. X. Wang

2014 ◽  
Vol 56 (12) ◽  
pp. 125006 ◽  
Author(s):  
J W Connor ◽  
R J Hastie ◽  
I Pusztai ◽  
P J Catto ◽  
M Barnes

2016 ◽  
Vol 23 (12) ◽  
pp. 122509 ◽  
Author(s):  
R. B. Zhang ◽  
X. Q. Lu ◽  
Q. H. Huang ◽  
J. Q. Dong ◽  
X. Y. Gong

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