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(EXP3/08) Alfvén Instabilities during ICRF Minority Heating in TFTR

S. Bernabei, M. G. Bell, R. Budny, D. Darrow, E. D. Fredrickson, J. C. Hosea, R. Majeski, E. Mazzucato, N. Gorelenkov1, C. K. Phillips, J. H. Rogers2, G. Schilling, J. R. Wilson, R. White, F. Zonca3, S. Zweben

Princeton Plasma Physics Laboratory, P.O. box 451, Princeton N.J. 08543
1 TRINITI, Troitsk, Moscow, Russia 142 092
2 Intevac Inc., 3550 Basset St., Santa Clara, Ca. 95054
3 Associazione EURATOM-ENEA, CRE 00044 Frascati, Italy

Abstract.  High power ICRF minority heating produces an energetic tail in the distribution function of the resonant ions. When the energy in this tail exceeds a certain threshold, various kinds of Alfvénic instabilities can be excited. In TFTR, it is found that modes whose frequencies decrease vs. time cause fast ion losses and in turn a reduced Rf heating efficiency, unlike the usual global TAE. The frequency decrease of the modes is found to correspond to a radial movement of t he mode itself: modelling shows that this feature causes an avalanche of fast ion losses due to a diffusion process. The frequency-decreasing modes play a fundamental role in the stabilization of the sawtooth and in its subsequent crash.

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IAEA 2001