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
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Feng Liu
Université Côte d’Azur & CASTOR/Inria Sophia-Antipolis, France
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Guido Huijsmans
CEA, IRFM, F-13108 Saint-Paul-Lez-Durance, France
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Alberto Loarte
ITER, ITER organization
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A.M. Garofalo
GA, US, GA, General Atomics, P.O. Box 85608, San Diego, California 92186-5608, USA, General Atomics
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Wayne Solomon
General Atomics, P.O. Box 85608, San Diego, California 92186-5608, USA, General Atomics
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Boniface Nkonga
Université Côte d’Azur & CASTOR/Inria Sophia-Antipolis, France
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Matthias Hoelzl
6Max Planck Institute for Plasma Physics, 85748 Garching, Germany, Max Planck Institute for Plasma Physics, Garching, Germany