β面涡壁相互作用及内开尔文波-流相互作用对深亚中尺度气旋的产生

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS
Charly de Marez, T. Meunier, Pauline Tedesco, P. L’Hégaret, X. Carton
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引用次数: 4

摘要

在本文中,我们研究了在理想情况下,使用亚中尺度和内波解析模型在β-平面上的涡壁相互作用。我们的结果为海洋中尺度涡旋向西部边界漂移的动力学提供了新的见解。我们表明,在相互作用中存在强烈的气旋/反气旋不对称,这与之前的研究相反:由于内部开尔文波-电流相互作用,反气旋不能沿壁面经向漂移。这种相互作用被证明是产生小型连贯亚中尺度气旋的有效机制,这些气旋可以传播数百公里进入海洋内部。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Vortex–wall interaction on the β-plane and the generation of deep submesoscale cyclones by internal Kelvin Waves–current interactions
ABSTRACT In this paper, we investigate the vortex–wall interaction on the β-plane, using a submesoscale and internal waves resolving model in an idealised context. Our results bring new insights on the dynamics of oceanic mesoscale eddies as they drift toward a western boundary. We show that there exists a strong cyclone/anticyclone asymmetry in the interaction, contrary to what was suggested in previous studies: anticyclones cannot drift meridionally along the wall because of internal Kelvin Waves–current interactions. This interaction is shown to be an efficient mechanism to generate small coherent submesoscale cyclones, which can travel hundreds of kilometres into the interior of the ocean.
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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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