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Parametric instability and wave turbulence driven by tidal excitation of internal waves

机译:潮汐激发驱动的参数不稳定性和波湍流   内波

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摘要

We investigate the stability of stratified fluid layers undergoinghomogeneous and periodic tidal deformation. We first introduce a local modelwhich allows to study velocity and buoyancy fluctuations in a Lagrangian domainperiodically stretched and sheared by the tidal base flow. While keeping thekey physical ingredients only, such a model is efficient to simulate planetaryregimes where tidal amplitudes and dissipation are small. With this model, weprove that tidal flows are able to drive parametric subharmonic resonances ofinternal waves, in a way reminiscent of the elliptical instability in rotatingfluids. The growth rates computed via Direct Numerical Simulations (DNS) are invery good agreement with WKB analysis and Floquet theory. We also investigatethe turbulence driven by this instability mechanism. With spatio-temporalanalysis, we show that it is a weak internal wave turbulence occurring at smallFroude and buoyancy Reynolds numbers. When the gap between the excitation andthe Brunt-V\"ais\"al\"a frequencies is increased, the frequency spectrum ofthis wave turbulence displays a -2 power law reminiscent of the high-frequencybranch of the Garett and Munk spectrum (Garrett & Munk 1979) which has beenmeasured in the oceans. In addition, we find that the mixing efficiency isaltered compared to what is computed in the context of DNS of stratifiedturbulence excited at small Froude and large buoyancy Reynolds numbers and isconsistent with a superposition of waves.
机译:我们研究了均质和周期性潮汐变形的分层流体层的稳定性。我们首先介绍一个局部模型,该模型可以研究潮汐基流在拉格朗日域中周期性拉伸和剪切的速度和浮力波动。虽然仅保留关键的物理成分,但这种模型可有效地模拟潮汐振幅和耗散较小的行星状态。通过该模型,我们证明了潮汐流能够驱动内部波的参数次谐波共振,从而使人联想到旋转流体中的椭圆形不稳定性。通过直接数值模拟(DNS)计算的增长率与WKB分析和Floquet理论非常吻合。我们还研究了由这种不稳定机制驱动的湍流。通过时空分析,我们发现它是在smallFroude和浮力雷诺数处发生的弱内部波湍流。当激发频率和Brunt-V'ais'al频率之间的差距增大时,该波湍流的频谱显示出-2幂定律,让人联想到Garett和Munk频谱的高频分支(Garrett和Munk(1979)(在海洋中进行了测量),此外,与在小Froude和大浮力雷诺数下激发的分层湍流DNS中计算的混合效率相比,混合效率有所变化,并且与波浪的叠加一致。

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