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Title: A kinetic theory of trapped-electron-driven drift wave turbulence in a sheared magnetic field

Journal Article · · Physics of Fluids B; (USA)
DOI:https://doi.org/10.1063/1.859957· OSTI ID:6390064
 [1]; ;  [2]
  1. Institute for Fusion Studies, University of Texas at Austin, Austin, Texas 78712 (US)
  2. Department of Physis B-019, University of California, San Diego, La Jolla, California 92093 (USA) General Atomics, Inc., San Diego, California 92186-9784 (USA)

A kinetic theory of collisionless and dissipative trapped-electron-driven drift wave turbulence in a sheared magnetic field is presented. Weak turbulence theory is employed to calculate the nonlinear electron and ion responses and to derive a wave kinetic equation that determines the nonlinear evolution of trapped-electron mode turbulence. The saturated fluctuation spectrum is calculated using the condition of nonlinear saturation. The turbulent transport coefficients ({ital D}, {chi}{sub {ital i}}, {chi}{sub {ital e}}), are, in turn, calculated using the saturated fluctuation spectrum. Because of the disparity in the three different radial scale lengths of the slab-like eigenmode: {Delta} (trapped-electron layer width), {ital x}{sub {ital t}} (turning point width), and {ital x}{sub {ital i}} (Landau damping point), {Delta}{lt}{ital x}{sub {ital t}}{lt}{ital x}{sub {ital i}}, it is found that ion Compton scattering rather than trapped-electron Compton scattering is the dominant nonlinear saturation mechanism. Ion Compton scattering transfers wave energy from short to long wavelengths where the wave energy is shear damped. As a consequence, a saturated fluctuation spectrum {vert bar}{phi}{vert bar}{sup 2}({ital k}{sub {theta}}){similar to}{ital k}{sup {minus}{alpha}}{sub {theta}} ({alpha}=2 and 3 for the dissipative and collisionless regimes, respectively) occurs for {ital k}{sub {theta}} {rho}{sub {ital s}}{lt}1 and is heavily damped for {ital k}{sub {theta}} {rho}{sub {ital s}}{gt}1. The predicted fluctuation level and transport coefficients are well below the mixing length'' estimate.

OSTI ID:
6390064
Journal Information:
Physics of Fluids B; (USA), Vol. 3:1; ISSN 0899-8221
Country of Publication:
United States
Language:
English