Gta. Huysmans et al., Modeling of diamagnetic stabilization of ideal magnetohydrodynamic instabilities associated with the transport barrier, PHYS PLASMA, 8(10), 2001, pp. 4292-4305
A new code, MISHKA-D (Drift MHD), has been developed as an extension of the
ideal magnetohydrodynamics (MHD) code MISHKA-1 in order to investigate the
finite gyroradius stabilizing effect of ion diamagnetic drift frequency, o
mega (*i), on linear ideal MHD eigenmodes in tokamaks in general toroidal g
eometry. The MISHKA-D code gives a self-consistent computation of both stab
le and unstable eigenmodes with eigenvalues \gamma\congruent to omega (*i)
in plasmas with strong radial variation in the ion diamagnetic frequency. T
est results of the MISHKA-D code show good agreement with the analytically
obtained omega*(i) spectrum and stability limits of the internal kink mode,
n/m=1/1, used as a benchmark case. Finite-n ballooning and low-n kink (pee
ling) modes in the edge transport barrier just inside the separatrix are st
udied for high confinement mode (H-mode) plasmas with the omega (*i) effect
included. The ion diamagnetic stabilization of the ballooning modes is fou
nd to be most effective for narrow edge pedestals. For low enough plasma de
nsity the omega (*i) stabilization can lead to a second zone of ballooning
stability, in which all the ballooning modes are stable for any value of th
e pressure gradient. For internal transport barriers typical of the Joint E
uropean Torus [JET, P. H. Rebut , Proceedings of the 10th International Con
ference, Plasma Physics and Controlled Nuclear Fusion, London (Internationa
l Atomic Energy Agency, Vienna, 1985), Vol. I, p. 11] optimized shear disch
arges, the stabilizing influence of ion diamagnetic frequency on the n=1 gl
obal pressure driven disruptive mode is studied. A strong radial variation
of omega (*i) is found to significantly decrease the stabilizing omega (*i)
effect on the n=1 mode, in comparison with the case of constant omega (*i)
estimated at the foot of the internal transport barrier. (C) 2001 American
Institute of Physics.