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Glossary

Resistive Wall Mode

A slowly growing kink that exploits the finite resistivity of the vacuum vessel wall to bypass what should be a hard stability limit.

Reviewed Last reviewed: 9 Aug 2026 · Category: Glossary

What Is a Resistive Wall Mode?

A resistive wall mode (RWM) is a global MHD instability that would be stabilized by a perfectly conducting wall but grows on the resistive timescale of the real wall surrounding the plasma. In ideal MHD a close-fitting superconducting shell can raise the pressure limit (the so-called "wall-stabilized" beta limit) well above the no-wall value. A real wall, however, has finite resistivity: eddy currents induced by the mode decay on a timescale τw = μ0σdδ, where σ is the wall conductivity, d its thickness, and δ its effective distance from the plasma. The RWM grows on roughly this timescale—seconds in a large tokamak—making it slow compared with ideal kinks but still fast enough to terminate a discharge.1

Relevance to High-Performance Operation

Advanced tokamak scenarios depend on operating above the no-wall beta limit to achieve high bootstrap-current fractions and economically attractive fusion power density. The RWM is the principal obstacle: unless it is actively controlled, the plasma cannot access the regime between the no-wall and ideal-wall stability boundaries.2

ITER's baseline scenario stays below the no-wall limit, but steady-state scenarios and virtually all compact-tokamak designs require RWM stabilization to reach their target beta values. The mode is therefore a gatekeeper for the economic viability of the tokamak concept.

Stabilization Techniques

Two broad strategies exist. Passive stabilization relies on plasma rotation: a toroidally rotating plasma interacts with the resistive wall through a rotationally induced phase shift that provides effective dissipation, converting the growing mode into a damped one. Experiments on DIII-D showed that a critical rotation threshold (typically a few percent of the Alfvén speed) is sufficient.3

Active feedback control uses external saddle coils driven by real-time magnetic sensors to apply a correction field that opposes the RWM perturbation. This approach has been demonstrated on DIII-D, NSTX, JT-60U, and KSTAR, and is the baseline strategy for devices where neutral-beam torque may be insufficient to maintain rotation.4

Kinetic effects—resonances between the slow RWM and thermal-ion or energetic-particle drift motions—provide additional damping and can raise the rotation threshold or even eliminate it, a finding with important implications for reactor designs where rotation drive is limited.

Sources

  1. A. Bondeson and D. J. Ward, "Stabilization of external modes in tokamaks by resistive walls and plasma rotation," Physical Review Letters, vol. 72, pp. 2709–2712, 1994.
  2. M. Okabayashi et al., "Active feedback stabilization of the resistive wall mode on the DIII-D device," Nuclear Fusion, vol. 45, pp. 1715–1731, 2005.
  3. S. A. Sabbagh et al., "Resistive wall mode stabilization and plasma rotation damping considerations for maintaining high beta plasma discharges in NSTX," Nuclear Fusion, vol. 46, pp. 635–644, 2006.
  4. J. W. Berkery et al., "The role of kinetic effects on resistive wall mode stability in NSTX and DIII-D," Physics of Plasmas, vol. 17, 082504, 2010.

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