Linear Gyrokinetic Analysis of High Poloidal Beta Discharge on DIII-D

POSTER

Abstract

Linear gyrokinetic simulations performed on kinetic equilibrium reconstructions of high poloidal beta DIII-D discharges show the features of the dominant micro-turbulent instabilities. In low-k range, ITG-like and KBM-like modes co-exist outside the large radius internal transport barrier (ITB) in the low pressure gradient region (rho=0.73) as dominant modes for different k_thetas. In these simulations, the ITG-like mode is very marginal to many parameters, e.g. beta, collisionality and ion temperature scale length. Some increase in these parameters will bring a conversion of this mode to KBM-like mode, which has out-of-phase parity in the parallel part of the vector potential. The linear growth rate of the KBM-like mode is proportional to plasma beta. Ion temperature gradient is the major driving force of this instability. In the steep gradient region of ITB, the KBM-like mode can still be seen unstable and the ITG-like mode changes to an electron mode. The comparison with turbulence measurement in experiment will also be presented.

Presenters

  • Siye Ding

    ORAU/ASIPP, ORAU/ASIPP, ASIPP

Authors

  • Siye Ding

    ORAU/ASIPP, ORAU/ASIPP, ASIPP

  • Joseph McClenaghan

    ORAU, General Atomics - San Diego

  • Andrea MV Garofalo

    General Atomics - San Diego, General Atomics

  • Gary M Staebler

    GA, General Atomics - San Diego

  • George R Mckee

    Univ of Wisconsin, Madison, Univ of Wisconsin, Madison, Univ of Wisconsin, Madison, University of Wisconsin–Madison, University of Wisconsin-Madison, University of Wisconsin - Madison, University of Wisconsin, Madison, Univ. of Wisconsin, Madison

  • Zheng Yan

    Univ of Wisconsin, Madison, University of Wisconsin–Madison, University of Wisconsin - Madison, University of Wisconsin, Madison

  • Wenfeng Guo

    ASIPP

  • Jinping Qian

    ASIPP

  • Xianzu Gong

    Institute of Plasma Physics, Chinese Academy of Sciences, ASIPP, Institute of Plasma Physics, Chinese Academy of Sciences, P.O. Box 1126, Hefei, Anhui 230031, People’s Republic of China

  • Chengkang Pan

    ASIPP