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Theory of mean poloidal flow generation by turbulence

Phys. Fluids B 3, 1626 (1991); doi:10.1063/1.859681

Issue Date: July 1991

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P. H. Diamond and Y.-B. Kim
Department of Physics, University of California, San Diego, La Jolla, California 92093
The mechanism for generation of mean poloidal flow by turbulence is identified and elucidated. Two methods of calculating poloidal flow acceleration are given and shown to yield predictions which agree. These methods link flow generation to the quasilinear radial current or the Reynolds stress <V-tilde rV-tilde theta>. It is shown that poloidal acceleration will occur if the turbulence supports radially propagating waves and if radial gradients in the turbulent Reynolds stress and wave energy density flux are present. In practice, these conditions are met in the tokamak edge region when waves propagate through the outermost closed flux surface or when convection cells with large radial correlation length are situated in steep gradient regions. The possible impact of these results on the theory of the L-->H transition is discussed. Physics of Fluids B: Plasma Physics is copyrighted by The American Institute of Physics.
History: Received 25 September 1990; accepted 1 March 1991
Permalink: http://dx.doi.org/10.1063/1.859681
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KEYWORDS and PACS

Keywords
PACS
  • 52.25.Gj
    The physics of plasmas and electric discharges Plasma properties Fluctuation phenomena
  • 52.35.Ra
    The physics of plasmas and electric discharges Waves, oscillations, and instabilities in plasma Plasma turbulence
  • 52.55.-s
    The physics of plasmas and electric discharges Plasma equilibrium and confinement
  • YEAR: 1990-91

PUBLICATION DATA

ISSN:
0899-8221 (print)   1089-7674 (online)
Publisher:
AIP is a member of CrossRef AIP

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