纯应变中均匀准地转位涡细丝

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Geophysical and Astrophysical Fluid Dynamics Pub Date : 2023-07-04 DOI:10.1080/03091929.2023.2232939
J. Reinaud
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引用次数: 0

摘要

准地转位涡的三维细丝是大气和海洋流动的一般特征。它们通常在三维准地转涡旋之间的强相互作用中产生。它们促成了光谱空间中熵的直接级联。这些细丝对应于剪切带。因此,它们可能对剪切不稳定性很敏感,类似于经典二维涡度带的开尔文-亥姆霍兹不稳定性。然而,它们经常受到由周围漩涡引起的紧张流动的影响。这种应变流动影响了它们的鲁棒性。本文着重研究了这种情况的一个简化模型。我们考虑了纯应变对均匀准地转位涡三维细丝的影响。我们首先考虑一种准静态情况,在这种情况下,假设应变很小,只影响线材的横截面形状,而不影响速度场。在这种情况下,我们解决了灯丝的线性稳定性,并展示了灯丝非线性演变的例子。然后我们考虑在纯应变下的线材的线性化动力学。我们特别关注在灯丝中观察到的最大微扰放大。我们得出结论,小到中等应变率是有效的防止大的扰动增长。然而,非线性效应可以导致弱应变细丝的卷起。
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Filaments of uniform quasi-geostrophic potential vorticity in pure strain
Three-dimensional filaments of quasi-geostrophic potential vorticity are generic features of atmospheric and oceanic flows. They are often generated during the strong interactions between three-dimensional quasi-geostrophic vortices. They contribute to a direct cascade of enstrophy in spectral space. These filaments correspond to shear zones. Therefore they may be sensitive to shear instabilities akin to the Kelvin–Helmholtz instability of the classical two-dimensional vorticity strip. They are, however, often subjected to a straining flow induced by the surrounding vortices. This straining flow affects their robustness. This paper focuses on a simplified model of this situation. We consider the effect of a pure strain on a three-dimensional filament of uniform quasi-geostrophic potential vorticity. We first consider a quasi-static situation where the strain, assumed small, only affects the cross-sectional shape of the filament, but not the velocity field. We address the linear stability of the filament in that context and also show examples of the filament's nonlinear evolution. We then consider the linearised dynamics of the filament in pure strain. In particular we focus on the maximum perturbation amplification observed in the filament. We conclude that small to moderate strain rates are efficient at preventing a large perturbation growth. Nonlinear effects can nevertheless leads to the roll-up of weakly strained filaments.
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来源期刊
Geophysical and Astrophysical Fluid Dynamics
Geophysical and Astrophysical Fluid Dynamics 地学天文-地球化学与地球物理
CiteScore
3.10
自引率
0.00%
发文量
14
审稿时长
>12 weeks
期刊介绍: Geophysical and Astrophysical Fluid Dynamics exists for the publication of original research papers and short communications, occasional survey articles and conference reports on the fluid mechanics of the earth and planets, including oceans, atmospheres and interiors, and the fluid mechanics of the sun, stars and other astrophysical objects. In addition, their magnetohydrodynamic behaviours are investigated. Experimental, theoretical and numerical studies of rotating, stratified and convecting fluids of general interest to geophysicists and astrophysicists appear. Properly interpreted observational results are also published.
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