Stability of filaments of uniform quasi-geostrophic potential vorticity

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS
J. Reinaud
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引用次数: 2

Abstract

We analyse the linear stability of filaments of uniform potential vorticity with a horizontal axis in a quasi-geostrophic flow. For a single filament, the situation corresponds to the simplest three-dimensional shear zone in a rapidly rotating, continuously stably stratified fluid. Yet, this has not been formally addressed to our knowledge. We show that the filament is sensitive to the Kelvin–Helmholtz instability for perturbations in a finite range of streamwise wavenumbers , similarly to the classical situation of a two-dimensional strip of uniform vorticity. We also analyse the stability of a jet formed by two parallel filaments of opposite PV whose axes are located on the same horizontal plane as well as the stability of “hetonic” filaments. Hetonic filaments consist of a pair of opposite PV filaments located at different heights. These can be sensitive to baroclinic instabilities over a wide range of longitudinal wavenumbers.
均匀准地转位涡细丝的稳定性
本文分析了准地转流中具有水平轴的均匀位涡细丝的线性稳定性。对于单个细丝,这种情况对应于快速旋转、连续稳定分层流体中最简单的三维剪切区。然而,据我们所知,这个问题还没有得到正式解决。我们表明,在有限范围的流向波数扰动下,灯丝对开尔文-亥姆霍兹不稳定性很敏感,类似于均匀涡度的二维条带的经典情况。我们还分析了由轴线在同一水平面上的两个相对PV的平行细丝形成的射流的稳定性以及“面面体”细丝的稳定性。Hetonic细丝由一对位于不同高度的相对PV细丝组成。它们可以对大范围纵波数范围内的斜压不稳定性敏感。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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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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