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漂移波湍流和非局域流的波动力学超出射线近似。

Wave kinetics of drift-wave turbulence and zonal flows beyond the ray approximation.

机构信息

Department of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08544, USA.

Princeton Plasma Physics Laboratory, Princeton, New Jersey 08543, USA.

出版信息

Phys Rev E. 2018 May;97(5-1):053210. doi: 10.1103/PhysRevE.97.053210.

DOI:10.1103/PhysRevE.97.053210
PMID:29906873
Abstract

Inhomogeneous drift-wave turbulence can be modeled as an effective plasma where drift waves act as quantumlike particles and the zonal-flow velocity serves as a collective field through which they interact. This effective plasma can be described by a Wigner-Moyal equation (WME), which generalizes the quasilinear wave-kinetic equation (WKE) to the full-wave regime, i.e., resolves the wavelength scale. Unlike waves governed by manifestly quantumlike equations, whose WMEs can be borrowed from quantum mechanics and are commonly known, drift waves have Hamiltonians very different from those of conventional quantum particles. This causes unusual phase-space dynamics that is typically not captured by the WKE. We demonstrate how to correctly model this dynamics with the WME instead. Specifically, we report full-wave phase-space simulations of the zonal-flow formation (zonostrophic instability), deterioration (tertiary instability), and the so-called predator-prey oscillations. We also show how the WME facilitates analysis of these phenomena, namely, (i) we show that full-wave effects critically affect the zonostrophic instability, particularly its nonlinear stage and saturation; (ii) we derive the tertiary-instability growth rate; and (iii) we demonstrate that, with full-wave effects retained, the predator-prey oscillations do not require zonal-flow collisional damping, contrary to previous studies. We also show how the famous Rayleigh-Kuo criterion, which has been missing in wave-kinetic theories of drift-wave turbulence, emerges from the WME.

摘要

非均匀漂移波湍流可以被建模为一种有效等离子体,其中漂移波充当量子样粒子,而环流速度则作为它们相互作用的集体场。这种有效等离子体可以用维格纳-莫约尔方程(WME)来描述,该方程将准线性波动动力学方程(WKE)推广到全波范围,即解决波长尺度问题。与由明显量子样方程控制的波不同,其 WME 可以从量子力学中借用,并且通常是已知的,漂移波的哈密顿量与传统量子粒子的哈密顿量非常不同。这导致了通常无法被 WKE 捕捉到的不寻常的相空间动力学。我们展示了如何用 WME 来正确地模拟这种动力学。具体来说,我们报告了环流形成(纬向流不稳定)、恶化(三级不稳定)和所谓的捕食者-猎物振荡的全波相空间模拟。我们还展示了 WME 如何促进对这些现象的分析,即:(i)我们表明全波效应对纬向流不稳定,特别是其非线性阶段和饱和,具有至关重要的影响;(ii)我们推导出三级不稳定增长率;(iii)我们证明,与以前的研究相反,在保留全波效应的情况下,捕食者-猎物振荡不需要环流碰撞阻尼。我们还展示了著名的 Rayleigh-Kuo 准则如何从 WME 中出现,而该准则在漂移波湍流的波动动力学理论中一直缺失。

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