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Numerical Simulations of Turbulent Trapping in the Weak Beam-Plasma Instability

机译:弱光束等离子体不稳定性中湍流俘获的数值模拟

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Numerical simulations of the weak beam-plasma instability were done in the turbulent regime where small-scale trapping is a dominent feature of the instability, a regime with behavior not predicted by quasilinear theory. It occurs when the trapping frequency nu = (k sup 2 D)/sup 1/3/ is larger than the growth rate gamma /sub k/ of the instability. The results of the simulations were compared with those of a specific model of the turbulence, the so-called ''turbulent trapping'' model, which gives precise formulas for the particle correlation functions, and predicts a growth rate well enhanced over the quasilinear value. It was found that the model gives accurate predictions for the correlation functions, and thus provides a good description of the turbulent structure of phase space. On the other hand, while growth rates were enhanced over the quasilinear values, the enhancements observed are smaller than expected from the quantitative predictions of the model. Further work is necessary to determine whether this discrepancy is a failing of the turbulent trapping model, or the result of the numerical limitations of our computational scheme. (ERA citation 11:042308)

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