INTERNAL DISRUPTIONS IN HELIOTRON E-ASTERISK

In Heliotron E [K. Uo, Nucl. Fusion 25, 1243 [1985)] shifted-in vacuum magnetic field configuration, the q profile varies from just above 2 at the magnetic axis to 0.4 at the plasma edge. For low-beta plasmas, resistive interchange modes are the dominant low-n instabilities at th e plasma core. They saturate at low fluctuation levels. Above a thresh old value, the ideal m/n = 2/1 modes become unstable. They can be reso nant or nonresonant modes depending on the value of q( 0). In either c ase, their nonlinear evolution leads to a sudden crash of the pressure within the r/a = 0.3 radius (sawtooth oscillation). When beta is incr eased further, the q = 2 surface moves out of the plasma, and the idea l m/n = 2/1 modes are effectively stabilized when q(0) < 1.85. As a re sult, the sawtooth oscillations are suppressed. (C) 1998 American Inst itute of Physics. [S1070-664X(98)03910-X].