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Three-wave coupling and weak turbulence of kinetic Alfven waves

机译:动力学阿尔夫文波的三波耦合和弱湍流

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The nonlinear dynamics of kinetic-Alfven-wave (KAW) turbulence is studied. Weak KAW turbulence induced by three-wave interaction among parallel-propagating KAWs has a direct energy cascade in the wavenumber domain k_(s⊥) > ρ_i~(-1) and an inverse cascade in the domain k_(s⊥) < ρ_i~(-1), resulting in Kolmogorov-type spectra. W_k ~ (k_z)~(-1/2)(k_⊥)~(-p), with exponents p = 4 and p = 3.5 respectively. The interaction including antiparallel-propagating KAWs, usually most effective, results in an inverse energy cascade over the whole k_⊥ range and p = 2 (at k_⊥ < ρ_i~(-1)) and p = 3.5 (for k_⊥ > ρ_i~(-1)) spectra. Three applications concerning KAW turbulence in flaring loops, in the Earth's magnetosphere and in tokamaks are considered. It is suggested that turbulent KAW spectra are common in space plasmas.
机译:研究了动力学阿尔夫文波(KAW)湍流的非线性动力学。由平行传播的KAW之间的三波相互作用引起的弱KAW湍流在波数域k_(s⊥)>ρ_i〜(-1)中具有直接能量级联,在波数域k_(s⊥)<ρ_i〜中具有反级联(-1),得到Kolmogorov型光谱。 W_k〜(k_z)〜(-1/2)(k_⊥)〜(-p),分别为p = 4和p = 3.5。包括反平行传播的KAW(通常最有效)在内的相互作用会导致在整个k_⊥范围内且p = 2(在k_⊥<ρ_i〜(-1)时)和p = 3.5(对于k_⊥>ρ_i)时能量级联反〜(-1))光谱。考虑了在燃烧环,地球磁层和托卡马克中有关KAW湍流的三个应用。建议在空间等离子体中常见湍流KAW谱。

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