Published May 2011
| Version v1
Journal article
Turbulence and bias-induced flows in simple magnetized toroidal plasmas
- 1. Department of Physics and Astronomy, Dartmouth College, Hanover, New Hampshire 03755 (United States)
- 2. Centre de Recherches en Physique des Plasmas - Ecole Polytechnique Federale de Lausanne, Association EURATOM-Confederation Suisse, CH-1015 Lausanne (Switzerland)
- 3. Department of Physics, Institute for Fusion Studies, University of Texas at Austin, Austin, Texas 78712 (United States)
- 4. Department of Physics, University of New Hampshire, Durham, New Hampshire 03824 (United States)
Description
Turbulence and bias-induced flows in simple magnetized toroidal plasmas are explored with global three-dimensional fluid simulations, focusing on the parameters of the Helimak experiment. The simulations show that plasma turbulence and transport in the regime of interest are dominated by the ideal interchange instability. The application of a bias voltage alters the structure of the plasma potential, resulting in the equilibrium sheared flows.These bias-induced vertical flows located in the gradient region appear to reduce the radial extent of turbulent structures,and thereby lower the radial plasma transport on the low field side.
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review. E, Statistical, Nonlinear, and Soft Matter Physics (Print)
- Journal Volume
- 83
- Journal Issue
- 5
- Journal Page Range
- p. 056406-056406.6
- ISSN
- 1539-3755
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43037834
- Subject category
- S42: ENGINEERING;
- Descriptors DEI
- FLOW MODELS; FLUTE INSTABILITY; PLASMA; PLASMA POTENTIAL; SHEAR; SIMULATION; THREE-DIMENSIONAL CALCULATIONS; TOROIDAL CONFIGURATION; TRANSPORT; TURBULENCE
- Descriptors DEC
- ANNULAR SPACE; CLOSED CONFIGURATIONS; CONFIGURATION; ELECTRIC POTENTIAL; INSTABILITY; MAGNETIC FIELD CONFIGURATIONS; MATHEMATICAL MODELS; PLASMA INSTABILITY; PLASMA MACROINSTABILITIES; SPACE
Optional Information
- Notes
- (c) 2011 American Institute of Physics