1999
DOI: 10.1109/27.763072
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Three-dimensional simulation of the vertical displacement event in tokamaks

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Cited by 4 publications
(2 citation statements)
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“…Plasma-Facing Components (PFCs) are faced magnificent electromagnetic (EM) loads during VDE disruption [1][2][3][4] , a significant event caused by the failure of magnetic field control [5][6][7] and the instability of the internal plasma excitation (magnetohydrodynamic, MHD perturbations [8][9] ). There are many reasons for the excitation of the disruptions, which are often accompanied by the increase of impurities density concentration in the core region (r/a=0) [10][11][12][13][14][15] , the increase of the E×B drift force [16][17][18] , the perturbation change of the plasma rotation velocity, and the turbulence caused by the instability of the magnetic fluids (MHD).…”
Section: Introductionmentioning
confidence: 99%
“…Plasma-Facing Components (PFCs) are faced magnificent electromagnetic (EM) loads during VDE disruption [1][2][3][4] , a significant event caused by the failure of magnetic field control [5][6][7] and the instability of the internal plasma excitation (magnetohydrodynamic, MHD perturbations [8][9] ). There are many reasons for the excitation of the disruptions, which are often accompanied by the increase of impurities density concentration in the core region (r/a=0) [10][11][12][13][14][15] , the increase of the E×B drift force [16][17][18] , the perturbation change of the plasma rotation velocity, and the turbulence caused by the instability of the magnetic fluids (MHD).…”
Section: Introductionmentioning
confidence: 99%
“…A prominent example of a fixed-boundary major disruption simulation showing a thermal quench is the kink-ballooning simulation of Park. 12 Free-boundary simulations, which have the computational boundary beyond the last-closed flux surface, have primarily been used for VDE disruptions 13,14 or studies of liquid walls, 15 where the dominant axisymmetric nature of the instability gives weak stochasticity ͑or none if only the n =0 component is kept͒. For more non-axisymmetric modes, accurate modeling of rapid parallel equilibration in three dimensions is required to resolve the distinction between the halo region and core region as the plasma evolves nonlinearly and becomes highly stochastic.…”
Section: Simulation Modelmentioning
confidence: 99%