The merger of two three-dimensional quasi-geostrophic baroclinic tripolar eddies

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS
J. Reinaud, X. Carton
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引用次数: 0

Abstract

We investigate the strong interaction between two baroclinic tripolar eddies in a three-dimensional, rapidly-rotating, continuously stratified flow under the quasi-geostrophic approximation. Each tripolar eddy consists of an anticyclonic central vortex with two oblate cyclonic vortices located above and below the anticyclone. The interaction depends on the vertical and horizontal offsets between the two tripolar eddies. For small and low PV oblate cyclones, each tripolar eddy alone is only weakly unstable to a baroclinic mode. The instability puts the three vortices out of alignment. Most of the eddy however survives the instability. When two tripolar eddies interact, their constituent vortices may merge. Merger occurs when the eddies are close enough together, and shows similarities with the merger of monopolar vortices. Vertically separated eddies do not align vertically. This suggests the importance of an external flow for the alignment, observed in the oceans, to occur. We finally show that the interaction between two tripolar eddies with intense oblate cyclones is very different and show similarities with the dynamics of dipolar baroclinic eddies known as hetons.
两个三维准地转斜压三极涡旋的合并
在准地转近似下,研究了三维快速旋转连续分层流中两个斜压三极涡旋之间的强相互作用。每个三极涡由一个反气旋中心涡和位于反气旋上方和下方的两个扁形气旋涡组成。这种相互作用取决于两个三极涡旋之间的垂直和水平偏移量。对于小的和低PV的扁形气旋,每个三极涡单独对斜压模态只有弱不稳定。这种不稳定性使三个漩涡不对齐。然而,大多数涡流在不稳定性中幸存下来。当两个三极涡旋相互作用时,它们的组成涡旋可能合并。当涡流足够靠近时,合并就会发生,并显示出与单极涡旋合并的相似之处。垂直分离的涡流不会垂直对齐。这表明,在海洋中观察到的这种排列发生时,外部流的重要性。我们最后表明,两个三极涡旋与强扁形气旋之间的相互作用是非常不同的,并显示出与被称为heton的偶极斜压涡旋的动力学相似之处。
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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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