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Theory of neoclassical resistivity-gradient-driven turbulence

Technical Report ·
OSTI ID:6636604
It is shown that rippling instabilities can tap the density gradient expansion free energy source through the density dependence of the neoclassical resistivity. Linear analyses show that the region where neoclassical rippling modes are significantly excited extends from the edge of the plasma to the region where ..nu../sub *e/ less than or equal to 1. Since these modes are non-dispersive, diamagnetic effects are negligible in comparison to the nonlinear decorrelation rate at saturation. Thus, the relevant regime is the 'strong turbulence' regime. The turbulent radial diffusivities of the temperature and the density are obtained as eigenvalues of the renormalized eigenmode equations at steady state. The density gradient acts to enhance the level of turbulence, compared to that driven by the temperature gradient alone. The saturated turbulent state is characterized by: current decoupling, the breakdown of Boltzmann relation, a radial mode scale of density fluctuations exceeding that of temperature fluctuations, implying that density diffusivity exceeds temperature diffusivity, and that density fluctuation levels exceed temperature fluctuation levels. Magnetic fluctuation levels are negligible. 29 refs., 1 fig.
Research Organization:
Texas Univ., Austin (USA). Inst. for Fusion Studies; California Univ., San Diego, La Jolla (USA). Dept. of Physics
DOE Contract Number:
FG05-80ET53088; FG03-88ER53275
OSTI ID:
6636604
Report Number(s):
DOE/ET/53088-356; IFSR-356; ON: DE89005391
Country of Publication:
United States
Language:
English