Reduced Critical Rotation for Resistive-Wall Mode Stabilization in a Near-Axisymmetric Configuration
Creators
- 1. Columbia University, New York, New York 10027 (United States)
- 2. General Atomics, San Diego, California 92186-5608 (United States)
- 3. Princeton Plasma Physics Laboratory, Princeton, New Jersey 08543-0451 (United States)
- 4. FARTECH, Inc., San Diego, California 92121 (United States)
- 5. Chalmers University of Technology, S-412 96 Goeteborg (Sweden)
Description
Recent DIII-D experiments with reduced neutral beam torque and minimum nonaxisymmetric perturbations of the magnetic field show a significant reduction of the toroidal plasma rotation required for the stabilization of the resistive-wall mode (RWM) below the threshold values observed in experiments that apply nonaxisymmetric magnetic fields to slow the plasma rotation. A toroidal rotation frequency of less than 10 krad/s at the q=2 surface (measured with charge exchange recombination spectroscopy using C VI) corresponding to 0.3% of the inverse of the toroidal Alfven time is sufficient to sustain the plasma pressure above the ideal MHD no-wall stability limit. The low-rotation threshold is found to be consistent with predictions by a kinetic model of RWM damping
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review Letters
- Journal Volume
- 98
- Journal Issue
- 5
- Journal Page Range
- p. 055001-055001.4
- ISSN
- 0031-9007
- CODEN
- PRLTAO
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 38106809
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- AXIAL SYMMETRY; CHARGE EXCHANGE; CONFIGURATION; DOUBLET-3 DEVICE; MAGNETIC FIELDS; MAGNETOHYDRODYNAMICS; PLASMA; PLASMA PRESSURE; RECOMBINATION; ROTATION; SPECTROSCOPY; STABILIZATION; WALLS
- Descriptors DEC
- CLOSED PLASMA DEVICES; FLUID MECHANICS; HYDRODYNAMICS; MECHANICS; MOTION; SYMMETRY; THERMONUCLEAR DEVICES; TOKAMAK DEVICES
Optional Information
- Notes
- (c) 2007 The American Physical Society