Published May 2011 | Version v1
Journal article

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

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