HHFW Heating and Current Drive Progress on NSTX

POSTER

Abstract

Operation of NSTX at B$_{T}$(0) = 0.55 T has increased the core power deposition and heating efficiency of the 30 MHz High Harmonic Fast Waves (HHFW) compared to previous B$_{T}$(0) $\le $ 0.45 T operation, particularly when launching longer parallel wavelengths. This improvement is attributed in part to moving the onset density at which the fast waves begin to propagate into the plasma to a point further from the wall [1]. At this field strength the HHFW power deposition at k$_{\vert \vert }$ = 7 m$^{-1}$ is comparable to that of k$_{\vert \vert }$ = 14 m$^{-1}$, and core heating at k$_{\vert \vert }$ = 3 m$^{-1}$ is now seen, albeit at lower efficiency. Comparisons with power deposition from full-wave models (AORSA) will be made and MSE measurements of driven current will be presented. \newline [1] see Invited Talk by J. Hosea, this conference.

*This research used resources of the National Center for Computational Sciences at Oak Ridge National Laboratory, managed by UT-Battelle, LLC, for the U.S. Dept. of Energy under contract DE-AC05-00OR22725

Authors

  • P.M. Ryan

    • ORNL
  • E.F. Jaeger

    • ORNL
  • J.B. Wilgen

    • ORNL
  • J.C. Hosea

    • PPPL
  • J.R. Wilson

    • PPPL
  • R.E. Bell

    • PPPL
  • S. Bernabei

    • PPPL
  • B.P. LeBlanc

    • PPPL
  • C.K. Phillips

    • PPPL
  • L. Delgado-Aparicio

    • John Hopkins University
  • K. Tritz

    • John Hopkins University
  • S. Sabbagh

    • Columbia University
  • H. Yuh

    • Nova Photonics