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Title: Transition from resistive-g to eta-i driven turbulence in stellarator systems

Technical Report ·
DOI:https://doi.org/10.2172/7055394· OSTI ID:7055394
 [1]; ;  [2]; ; ;  [3]
  1. ENEA, Frascati (Italy). Centro Ricerche Energia
  2. Texas Univ., Austin, TX (USA). Inst. for Fusion Studies
  3. Kyoto Univ., Uji (Japan). Plasma Physics Lab.

By an electromagnetic incompressible two fluid model describing both ion temperature gradient drift modes ({eta}{sub i} modes) and resistive interchange modes (g modes), a new type of {eta}{sub i} mode is studied in cylindrical geometry including magnetic shear and an averaged curvature of Heliotron/Torsatron. This {eta}{sub i} mode is destabilized by the coupling to the unstable g mode. Finite plasma pressure beta increases the growth rate of this mode and the radial mode width also increases with plasma pressure beta indicating large anomalous transport in the Heliotron/Torsatron configuration. The transport from {eta}{sub i} mode exceeds that from resistive g when the mean-free-path exceeds the machine circumference. For plasma beta above two to three times the Suydam limit the m = 1/n = 1 growth rate increases from the {eta}{sub i} mode value to the MHD value. 13 refs., 5 figs.

Research Organization:
Texas Univ., Austin, TX (USA). Inst. for Fusion Studies
Sponsoring Organization:
DOE/ER
DOE Contract Number:
FG05-80ET53088
OSTI ID:
7055394
Report Number(s):
DOE/ET/53088-417; IFSR-417; ON: DE90009382; TRN: 90-010524
Country of Publication:
United States
Language:
English