Drift stabilization of internal resistive-wall modes in tokamaks

Abstract

The problem of drift stabilization of the internal resistive-wall modes (RWMs) in tokamaks is theoretically investigated. The basic assumption of the model is that, when the drift effects are neglected, these modes are unstable in the absence of a conducting wall and stable in the presence of a close-fitting perfectly conducting wall. In the former case, the instability condition is expressed as Δ′_∞>0, where Δ′_∞ is the matching parameter calculated under the assumption that the wall is removed to infinity. In the latter case, one has Δ ^′_W <0, where Δ ^′_W is the external matching parameter of tearing modes calculated assuming a perfectly conducting wall at the plasma boundary. In the case with a resistive wall, the relevant parameter can be either Δ′_∞ or Δ ^′_W , depending on whether the value of the dimensionless parameter ωτ_s/2m is small or large, respectively (here ω is the mode frequency, τ_s is the resistive time constant of the wall, and m is the poloidal mode number). In the presence of drift effects, the mode frequency ω is approximately equal to the electron drift frequency, ω≈ω_*e . The value of the parameter ω_*e τ_s/2m, which therefore determines the behavior of internal RWMs, is estimated for several existing tokamaks, namely, AUG (ASDEX-Upgrade), DIII-D, JET, TFTR, and JT-60U, as well as for the projected ITER-FEAT. It is shown that, although drift effects do not stabilize internal RWMs in current devices, they should be efficient in suppressing these modes in reactor-grade tokamaks.