大型合并涡中心的小尺度涡的形成

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Geophysical and Astrophysical Fluid Dynamics Pub Date : 2022-05-25 DOI:10.1080/03091929.2022.2074983
Erwan Oulhen, J. Reinaud, X. Carton
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引用次数: 1

摘要

详细研究了两个表面准地转涡旋的合并。当两个涡旋在合并过程中向对方坍缩时,它们将外部锋面困在它们之间;这些锋面被插入到最终合并的涡旋中,在那里它们形成一个中心的、几乎平行的、剪切的速度带,对正压不稳定性很敏感。结果,这条带分裂成一条小漩涡的小巷。随后,这些小涡可能会在大合并涡的核心进行合并并扩大规模。被困小涡的数量相应减少。最后,留下一两个小漩涡。利用地表准地转方程的数值模型对这些过程进行了分析。探讨了该过程对初始涡特性的敏感性。这一问题与具有中心间隙的温度直线带的不稳定性有相似之处。讨论了这一问题在海洋中的应用。
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Formation of small-scale vortices in the core of a large merged vortex
The merger of two surface quasi-geostrophic vortices is examined in detail. As the two vortices collapse towards each other in the merging process, they trap their external fronts between them; these fronts are inserted into the final merged vortex, where they form a central, nearly parallel, sheared velocity strip, sensitive to barotropic instability. As a result, this strip breaks up into an alley of small vortices. Subsequently, these small vortices may undergo merger and grow in size in the core of the large merged vortex. The number of small trapped vortices decreases correspondingly. Finally, a single or two small vortices remain. These processes are analysed using a numerical model of the surface quasi-geostrophic equations. The sensitivity of this process to the initial vortex characteristics is explored. A parallel is drawn between this problem and the instability of a rectilinear strip of temperature with a central gap. The application of this problem to the Ocean is discussed.
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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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