Simulating the effect of external helical magnetic fields on MHD stability of tokamak plasma

1999 ◽  
Vol 10 (4) ◽  
pp. 329-337
Author(s):  
Liu Hsiu-tsian ◽  
A. M. Popov
Keyword(s):  
Magnetic Fields ◽  
Tokamak Plasma ◽  
Mhd Stability

Vertical MHD Stability of the T-15M Tokamak Plasma

2003 ◽  
Vol 11 (4) ◽  
pp. 219-227 ◽  
Author(s):  
E. N. Bondarchuk ◽  
YU. N. Dnestrovskij ◽  
V. M. Leonov ◽  
I. I. Maksimova ◽  
D. YU. Sychugov ◽  
...  
Keyword(s):  
Tokamak Plasma ◽  
Mhd Stability

Observation of disruptions in tokamak plasma under the influence of resonant helical magnetic fields

1996 ◽  
Vol 18 (7) ◽  
pp. 807-821 ◽  
Author(s):  
M. S. T. Araújo ◽  
A. Vannucci ◽  
I. L. Caldas
Keyword(s):  
Magnetic Fields ◽  
Tokamak Plasma

Analysis on MHD Stability of Free Surface Jet flow in a Gradient Magnetic Fields

2004 ◽  
Vol 6 (3) ◽  
pp. 2301-2306
Author(s):  
Xu Zengyu ◽  
Kang Weishan ◽  
Pan Chuanjie
Keyword(s):  
Free Surface ◽  
Magnetic Fields ◽  
Jet Flow ◽  
Mhd Stability ◽  
Surface Jet

Calculated Coronal Magnetic Fields and Their Comparison with the Coronal Structures as Observed during Five Solar Eclipses

1994 ◽  
Vol 144 ◽  
pp. 559-564
Author(s):  
P. Ambrož ◽  
J. Sýkora
Keyword(s):  
Magnetic Field ◽  
Solar Cycle ◽  
Magnetic Fields ◽  
Solar Corona ◽  
Coronal Magnetic Field ◽  
Coronal Magnetic Fields ◽  
Solar Eclipses ◽  
Coronal Structures

AbstractWe were successful in observing the solar corona during five solar eclipses (1973-1991). For the eclipse days the coronal magnetic field was calculated by extrapolation from the photosphere. Comparison of the observed and calculated coronal structures is carried out and some peculiarities of this comparison, related to the different phases of the solar cycle, are presented.

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