Parametric dependence and control of 3D helical structures in MST

ORAL

Abstract

MST plasmas with a central 3D helical structure are now routinely achievable. As in RFX-mod, the stellarator-like structure arises in otherwise toroidally axisymmetric plasmas when the innermost-resonant m = 1 tearing mode grows to large amplitude and dominates the core-resonant-mode spectrum. The tearing mode spectrum in MST varies strongly with toroidal plasma current. Peaked spectra with a helical structure occur most reliably at high Ip (0.6 MA), while at low Ip (0.2 MA), the spectra are quite flat. This trend is like that in RFX-mod and may reflect a dependence on the Lundquist number. Preliminary MST data also show that manipulation of the inductive electric field has a significant impact, driving the dominant mode to large amplitude more robustly, and reducing the other modes. At high Ip, Te(0) $>$ 1 keV with a possible several-fold increase in the energy confinement time. Supported by USDOE.

Authors

  • B.E. Chapman

  • D.J. Den Hartog

  • J.A. Goetz

  • M.B. McGarry

  • E. Parke

  • J.A. Reusch

  • J.S. Sarff

    • UW-Madison
  • W.F. Bergerson

  • D.L. Brower

  • W.X. Ding

  • L. Lin

    • UCLA
  • F. Auriemma

  • S. Cappello

  • P. Franz

  • P. Innocente

  • R. Lorenzini

  • E. Martines

  • B. Momo

  • P. Piovesan

  • M. Puiatti

  • M. Spolaore

  • D. Terranova

  • P. Zanca

    • Consorzio RFX