Gas puff imaging diagnostic on NSTX-U$

POSTER

Abstract

The first results and plans for the gas puff imaging (GPI) diagnostic on NSTX-U will be described. The GPI optical efficiency has been improved by about x10 using a new fiber bundle and interference filter, and the new optics has a zoom lens which can potentially resolve turbulence below the ion gyroradius scale. Experiments are planned to study high-k edge turbulence, correlations of edge turbulence with the SOL heat flux width, and the trigger mechanism of the L-H transition. A second fast camera is planned to view the GPI gas cloud from across the machine, which can potentially measure the field line pitch by simultaneously viewing individual field-aligned blob filaments in the radial vs. poloidal (GPI) and toroidal vs. poloidal (second camera) directions. An incoming collaboration from MIT will bring a 9x10 pixel APD-based detector array from Alcator C-Mod to NSTX-U, initially for faster and more sensitive imaging of the existing GPI gas puff. New results and further diagnostic plans will be described.

*This work was supported by USDOE Contracts #DE-AC02-09CH11466, DE-SC0014264, and DE-AC52-07NA27344.

Authors

  • Stewart Zweben

    • PPPL
    • Princeton Plasma Physics Laboratory
  • F. Scotti

    • LLNL
  • D.L. Stotler

    • PPPL
  • A. Diallo

    • PPPL
  • N. Mandell

    • PPPL
  • J.L. Terry

    • MIT
  • W. Han

    • MIT