两个三维准地转涡旋的排列

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Geophysical and Astrophysical Fluid Dynamics Pub Date : 2019-08-25 DOI:10.1080/03091929.2019.1653462
J. Reinaud, X. Carton
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引用次数: 4

摘要

我们考虑两个高宽比为h/r的准地转涡旋之间的相互作用,它们位于两个不同的垂直水平。我们调查这些结构是否自然排列。当涡旋在不同的垂直水平面上时,这种排列有助于增加海洋中尺度涡旋的体积。另一种生长机制是具有共同垂直水平的涡旋的合并。我们证明了存在所谓的平衡状态,其中涡旋几乎倾斜排列。大多数长旋涡()的平衡点在参数空间的一个非常窄的区域内是稳定的。然而,这种不稳定性通常是非破坏性的。扁涡对如果在水平方向上有适度的偏移,也可能处于不稳定的平衡状态。在这种情况下,这种不稳定性可能导致丝状潜在涡量从涡旋上脱落。这种潜在涡度的脱落可能导致主要结构的进一步排列。
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The alignment of two three-dimensional quasi-geostrophic vortices
We consider the interaction between two quasi-geostrophic vortices of height-to-width aspect ratio h/r, lying at two different vertical levels. We investigate whether such structures naturally align. In the case the vortices occupy distinct yet contiguous vertical levels, such an alignment can contribute to the growth in volume of oceanic mesoscale vortices. The other growth mechanism is the merger of vortices sharing common vertical levels. We show that there exist titled equilibrium states where vortices nearly align slantwise. Most equilibria for prolate vortices ( ) are stable apart in a very narrow region of the parameter space. The instability is however normally non-destructive. Pairs of oblate vortices may also be in an unstable equilibria if they are moderately offset in the horizontal direction. In this case, the instability may result in the shedding of filamentary potentially vorticity away from the vortices. This shedding of potential vorticity may result in the further alignment of the main structures.
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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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