Influence of 3D magnetic fields on turbulence at the L-H transition and across magnetic islands in DIII-D

POSTER

Abstract

Measurements of long-wavelength density fluctuations using beam emission spectroscopy (BES) reveal the significant impact of 3D magnetic fields on turbulence amplitudes and characteristics. Fluctuations are measured across an applied static m,n $=$ 2,1 magnetic island that is rotated toroidally through the BES sightlines, providing quasi-3D measurement capability. A single unstable broadband turbulence mode is observed near the O-point, but near the X-point, this mode is accompanied by a second mode propagating in the opposite direction; fluctuation amplitudes are also much higher near the X-point than the O-point. 2D fluctuations are also measured in the L-mode edge leading up to L-H transitions with applied resonant and non-resonant magnetic perturbations. Normalized fluctuation amplitudes are \textasciitilde 4 times larger with resonant fields than with non-resonant fields. Additionally, dual counter-propagating modes are observed with resonant fields, while only a single mode is observed with non-resonant fields. These measurements may reveal how magnetic perturbations raise the L-H power threshold by altering turbulence-flow dynamics leading up to the transition.

Authors

  • Matt Kriete

    University of Wisconsin-Madison

  • G.R. Mckee

    UW-Madison, University of Wisconsin-Madison, UWisc, Madison, WI, Univ of Wisconsin, Madison, UWM

  • Raymond Fonck

    University of Wisconsin-Madison

  • David Smith

    University of Wisconsin-Madison

  • Zheng Yan

    UW-Madison, University of Wisconsin-Madison, UWisc, Madison, WI, Univ of Wisconsin, Madison, University of Wisconsin Madison

  • Lucas Morton

    ORAU, Oak Ridge Associated Universities

  • Morgan Shafer

    Oak Ridge National Laboratory

  • Lothar Schmitz

    UCLA, University of California Los Angeles, UCLA, Los Angeles, CA, Univ of California - Los Angeles