Kinetic Effects of Energetic Particles on Resistive MHD Stability
Creators
- 1. Department of Physics and Engineering Physics, University of Tulsa, 800 South Tucker Drive, Tulsa, Oklahoma 74104 (United States)
- 2. Plasma Science and Innovation Center, University of Washington, Seattle, Washington 98195 (United States)
Description
We show that the kinetic effects of energetic particles can play a crucial role in the stability of the m/n=2/1 tearing mode in tokamaks (e.g., JET, JT-60U, and DIII-D), where the fraction of energetic particle βfrac is high. Using model equilibria based on DIII-D experimental reconstructions, the nonideal MHD linear stability of cases unstable to the 2/1 mode is investigated including a δf particle-in-cell model for the energetic particles coupled to the nonlinear 3D resistive MHD code NIMROD[C. C. Kim et al., Phys. Plasmas 15, 072507 (2008)]. It is observed that energetic particles have significant damping and stabilizing effects at experimentally relevant β, βfrac, and S, and excite a real frequency of the 2/1 mode. Extrapolation of the results is discussed for implications to JET and ITER, where the effects are projected to be significant
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review Letters
- Journal Volume
- 102
- Journal Issue
- 13
- Journal Page Range
- p. 135001-135001.4
- ISSN
- 0031-9007
- CODEN
- PRLTAO
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 40054538
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- DOUBLET-3 DEVICE; EXTRAPOLATION; ITER TOKAMAK; JT-60U TOKAMAK; MAGNETOHYDRODYNAMICS; NONLINEAR PROBLEMS; TEARING INSTABILITY
- Descriptors DEC
- CLOSED PLASMA DEVICES; FLUID MECHANICS; HYDRODYNAMICS; INSTABILITY; MATHEMATICAL SOLUTIONS; MECHANICS; NUMERICAL SOLUTION; PLASMA INSTABILITY; PLASMA MACROINSTABILITIES; THERMONUCLEAR DEVICES; THERMONUCLEAR REACTORS; TOKAMAK DEVICES; TOKAMAK TYPE REACTORS
Optional Information
- Notes
- (c) 2009 The American Physical Society