scholarly journals Plasma rotation and rf heating in DIII-D

1999 ◽  
Author(s):  
J. S. deGrassie ◽  
D. R. Baker ◽  
K. H. Burrell ◽  
C. M. Greenfield ◽  
Y. R. Lin-Liu ◽  
...  
Keyword(s):  
2019 ◽  
Vol 55 (6) ◽  
pp. 302-304 ◽  
Author(s):  
Sen Wan ◽  
Changqing Jiang ◽  
Jianqi Ding ◽  
Luming Li
Keyword(s):  

2014 ◽  
Vol 21 (6) ◽  
pp. 062502 ◽  
Author(s):  
L. J. Zheng ◽  
M. T. Kotschenreuther ◽  
P. Valanju

2014 ◽  
Author(s):  
J. P. Lee ◽  
M. Barnes ◽  
R. R. Parker ◽  
J. E. Rice ◽  
F. I. Parra ◽  
...  
Keyword(s):  

1976 ◽  
Vol 16 (3) ◽  
pp. 419-426 ◽  
Author(s):  
R.J. Hawryluk ◽  
S.L. Davis ◽  
J.A. Schmidt

1979 ◽  
Vol 19 (8) ◽  
pp. 1073-1083 ◽  
Author(s):  
V.S. Chan ◽  
S.C. Chiu ◽  
G.E. Guest ◽  
R.W. Harvey ◽  
T. Ohkawa

1978 ◽  
Vol 41 (3) ◽  
pp. 201-201
Author(s):  
S. Suckewer ◽  
R. J. Hawryluk
Keyword(s):  

Author(s):  
shuyu Zheng ◽  
Debing Zhang ◽  
Erbing Xue ◽  
Limin Yu ◽  
Xianmei Zhang ◽  
...  

Abstract High poloidal beta scenarios with favorable energy confinement (β_p~1.9, H_98y2~1.4) have been achieved on Experimental Advanced Superconducting Tokamak (EAST) using only radio frequency waves heating. Gyrokinetic simulations are carried out with experimental plasma parameters and tokamak equilibrium data of a typical high β_p discharge by the GTC code. Linear simulations show that electron temperature scale length and electron density scale length destabilize the turbulence, collision effects stabilize the turbulence, and the instability propagates in the electron diamagnetic direction. These indicate that the dominant instability in the core of high β_p plasma is collisionless trapped electron mode. Ion thermal diffusivities calculated by nonlinear gyrokinetic simulations are consistent with the experimental value, in which the electron collision effects play an important role. Further analyses show that instabilities with k_θ ρ_s>0.38 are suppressed by collision effects and collision effects reduce the radial correlation length of turbulence, resulting in the suppression of the turbulence.


Author(s):  
Eduardo Lascas Neto ◽  
Jonathan P Graves ◽  
Madhusudan Raghunathan ◽  
Cristian Sommariva ◽  
David Pfefferlé

Abstract Strongly peaked tungsten accumulation is a common feature of high performance plasma scenarios in JET with the ITER-like wall, particularly during MHD activity induced by m⁄n = 1⁄1 continuous modes. This study investigates the effect of 1⁄1 long living internal kink modes on heavy impurity transport in the presence of strong flows and NTV ambipolar electric field. A novel formulation which includes these effects is presented and applied in the VENUS-LEVIS code in order to follow tungsten ions in a saturated JET-like 1⁄1 internal kinked toroidally rotating plasma configuration. The synergy between 3D magnetic fields, strong flows and NTV is seen to cause tungsten accumulation in contrast to what is observed in similar axisymmetric configurations. Rapid inward transport of impurities in JET plasmas following the triggering of continuous 1⁄1 modes is explained by the work presented here, and we use the same theory to postulate why outward transport can occur in kinked ASDEX-U plasmas.


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