Nonlinear MHD study on the influence of E\texttimes B flow in QH-mode plasma of DIII-D

ORAL

Abstract

In~QH-mode experiments with zero-net NBI torque show that there remains~a finite~E\texttimes B rotation in the pedestal region implying that a minimum~E\texttimes B flow or flow shear is required for the plasma to develop the Edge Harmonic Oscillation (EHO), which is a saturated KPM (kink-peeling mode)~characteristic of the QH-mode. To understand the roles of E\texttimes B flow and its shear in the saturation of KPMs,~non-linear MHD simulations~of DIII-D QH-mode plasmas including toroidal mode numbers n $=$ 0 to 10 with different E\texttimes B rotation speed have been performed. These simulation show that ExB~rotation strongly stabilizes high-n modes but destabilizes low-n modes (particularly the~n$=$2 mode) in the linear growth phase, which is consistent~experimental observations and previous linear MHD modelling.

Authors

  • Feng Liu

    Université Côte d’Azur & CASTOR/Inria Sophia-Antipolis, France

  • Guido Huijsmans

    CEA, IRFM, F-13108 Saint-Paul-Lez-Durance, France

  • Alberto Loarte

    ITER, ITER organization

  • A.M. Garofalo

    GA, US, GA, General Atomics, P.O. Box 85608, San Diego, California 92186-5608, USA, General Atomics

  • Wayne Solomon

    General Atomics, P.O. Box 85608, San Diego, California 92186-5608, USA, General Atomics

  • Boniface Nkonga

    Université Côte d’Azur & CASTOR/Inria Sophia-Antipolis, France

  • Matthias Hoelzl

    6Max Planck Institute for Plasma Physics, 85748 Garching, Germany, Max Planck Institute for Plasma Physics, Garching, Germany