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Magnetohydrodynamically generated velocities in confined plasma

Journal Article · · Physics of Plasmas
DOI:https://doi.org/10.1063/1.4918774· OSTI ID:22408323
 [1];  [2];  [3]
  1. LMFA, CNRS, École Centrale de Lyon, Écully (France)
  2. M2P2, CMI, CNRS, Aix-Marseille Université, Marseille (France)
  3. Department of Physics and Astronomy, Dartmouth College, Hanover, New Hampshire 03755 (United States)
We investigate by numerical simulation the rotational flows in a toroid confining a conducting magnetofluid in which a current is driven by the application of externally supported electric and magnetic fields. The computation involves no microscopic instabilities and is purely magnetohydrodynamic (MHD). We show how the properties and intensity of the rotations are regulated by dimensionless numbers (Lundquist and viscous Lundquist) that contain the resistivity and viscosity of the magnetofluid. At the magnetohydrodynamic level (uniform mass density and incompressible magnetofluids), rotational flows appear in toroidal, driven MHD. The evolution of these flows with the transport coefficients, geometry, and safety factor are described.
OSTI ID:
22408323
Journal Information:
Physics of Plasmas, Journal Name: Physics of Plasmas Journal Issue: 4 Vol. 22; ISSN PHPAEN; ISSN 1070-664X
Country of Publication:
United States
Language:
English