Published March 2005 | Version v1
Journal article

Reduced intermittency in the magnetic turbulence of reversed field pinch plasmas

  • 1. Department of Physics and Center for Magnetic Self-Organization in Astrophysical and Laboratory Plasmas, University of Wisconsin, 1150 University Avenue, Madison, Wisconsin 53706 (United States)
  • 2. Consorzio RFX, Associazione EURATOM-ENEA sulla Fusione, Corso Stati Uniti, 4 35127 Padova (Italy) and Dipartimento di Fisica G. Galilei, Universitat di Padova, 35131 Padova (Italy)
  • 3. Consorzio RFX, Associazione EURATOM-ENEA sulla Fusione, Corso Stati Uniti, 4 35127 Padova (Italy)

Description

The statistical temporal properties of broadband magnetic turbulence in the edge of reversed field pinch (RFP) plasmas are significantly altered when global magnetohydrodynamic tearing modes and magnetic relaxation are reduced. Standard RFP plasmas, having relatively large tearing fluctuations, exhibit broadband intermittent bursts of magnetic fluctuations in the bandwidth f<1.5 MHz. When the global tearing is reduced via parallel current drive in the edge region, the magnetic turbulence is much less intermittent and has statistical behavior typical of self-similar turbulence (like that expected in self-organized criticality systems). A connection between intermittency and long wavelength plasma instabilities is therefore implied

Additional details

Identifiers

Publishing Information

Journal Title
Physics of Plasmas
Journal Volume
12
Journal Issue
3
Journal Page Range
p. 030701-030701.4
ISSN
1070-664X
CODEN
PHPAEN

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
37014359
Subject category
S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
Descriptors DEI
BOUNDARY LAYERS; FLUCTUATIONS; MAGNETOHYDRODYNAMICS; PLASMA; REVERSE-FIELD PINCH; TEARING INSTABILITY; TURBULENCE
Descriptors DEC
FLUID MECHANICS; HYDRODYNAMICS; INSTABILITY; LAYERS; MECHANICS; PINCH EFFECT; PLASMA INSTABILITY; PLASMA MACROINSTABILITIES; VARIATIONS

Optional Information

Notes
(c) 2005 American Institute of Physics