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.

*US DOE under DE-FC02-04ER54698

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