Role of subdominant stable modes in plasma microturbulence
- 1. University of Wisconsin-Madison, Madison, Wisconsin 53706 (United States)
- 2. Max-Planck-Institut fuer Plasmaphysik, EURATOM Association, 85748 Garching (Germany)
- 3. Lawrence Livermore National Laboratory, Livermore, California 94550 (United States)
Description
In gyrokinetic simulations, thousands of degrees of freedom are available to contribute to the fluctuation spectrum. For wavevectors with a single linear instability, the unstable eigenmode accounts for only one of these degrees of freedom. Little has been known about the role of the remaining fluctuations in the turbulent dynamics. In this paper, these fluctuations are characterized as modes in mode decompositions of gyrokinetic distribution functions from nonlinear simulations. This analysis reveals the excitation of a hierarchy of damped modes at the same perpendicular scales as the driving instabilities. Two effects of these subdominant modes are described: First, these damped modes define a potent energy sink, creating a situation where energy drive and energy dissipation peak at the same perpendicular scales. Second, damped modes with tearing parity (even parity about the outboard midplane for A fluctuations) are driven to significant amplitudes and facilitate the development of magnetic stochasticity in electromagnetic gyrokinetic simulations.
Additional details
Identifiers
- DOI
- 10.1063/1.3563536;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 18
- Journal Issue
- 5
- Journal Page Range
- p. 055706-055706.11
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43016866
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- DISTRIBUTION FUNCTIONS; FLUCTUATIONS; PLASMA; PLASMA SIMULATION; TEARING INSTABILITY; TURBULENCE
- Descriptors DEC
- FUNCTIONS; INSTABILITY; PLASMA INSTABILITY; PLASMA MACROINSTABILITIES; SIMULATION; VARIATIONS
Optional Information
- Notes
- (c) 2011 American Institute of Physics