Singular Vortices on a Beta-Plane: A Brief Review and Recent Results

IF 0.7 Q4 OCEANOGRAPHY Physical Oceanography Pub Date : 2020-12-01 DOI:10.22449/1573-160x-2020-6-659-676
G. Reznik, S. Kravtsov
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引用次数: 2

Abstract

Purpose. This paper briefly reviews the theory of singular vortices (SV) on a beta-plane. Methods and Results : The primary focus of the paper is on a long-term evolution of an individual SV: the governing equations and integrals of motion are given, the algorithm of numerical implementation of these equations for investigation of such an evolution is described, and the results of some numerical experiments are presented. It is shown that the vortex evolution consists of two stages. At an initial (quasi-linear) stage, the near-field radiation of Rossby waves by the vortex produces, near the vortex, a non-stationary secondary dipole – the beta-gyres – which forces the vortex to move (a cyclone drifts northwestward, an anticyclone – southwestward). At the next (nonlinear) stage, the far-field radiation of Rossby waves and self-interactions within the regular component of the motion become of importance. A singular cyclone (anticyclone) migrates slowly into the anticyclonic (cyclonic) beta-gyre; the SV and the beta-gyre form a compact vortex pair which continues to move northwestward (southwestward). As this process takes place, the cyclonic (anticyclonic) beta-gyre gradually drifts away from and ceases to affect the SV, while the SV starts to interact with the Rossby waves it radiated previously, which results in oscillations of its translation speed. The duration of the quasi-linear stage rapidly increases with an increasing intensity of the SV; for vortices of small or moderate intensity, this stage ends rapidly and gives way to the nonlinear stage. The first phenomenological description of the nonlinear stage of a singular monopole’s evolution appeared in our recent work on the dynamics of the SV on a beta-plane. Conclusions : The theory of singular vortices on a beta-plane developed here significantly broadens our understanding of the evolution and dynamics of localized geophysical vortices which play an important role in the large-scale circulation of the ocean and atmosphere.
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β平面上的奇异涡旋:简评和最近的结果
意图本文简要回顾了β平面上奇异涡的理论。方法和结果:本文的主要焦点是单个SV的长期演化:给出了运动的控制方程和积分,描述了这些方程的数值实现算法,以研究这种演化,并给出了一些数值实验的结果。结果表明,旋涡的演化分为两个阶段。在初始(准线性)阶段,涡旋对罗斯比波的近场辐射在涡旋附近产生一个非平稳的二次偶极子——β涡旋——迫使涡旋移动(气旋向西北漂移,反气旋向西南漂移)。在下一个(非线性)阶段,罗斯比波的远场辐射和运动规则分量内的自相互作用变得至关重要。一个单一的气旋(反气旋)缓慢迁移到反气旋(气旋)贝塔环流中;SV和β-涡旋形成一对紧凑的涡旋,并继续向西北方向(西南方向)移动。随着这一过程的发生,气旋(反气旋)β涡旋逐渐远离SV并停止影响SV,而SV开始与之前辐射的Rossby波相互作用,这导致其平移速度振荡。准线性阶段的持续时间随着SV强度的增加而迅速增加;对于强度较小或中等的旋涡,这一阶段迅速结束,并让位给非线性阶段。奇异单极子演化的非线性阶段的第一个现象学描述出现在我们最近关于β平面上SV动力学的工作中。结论:这里发展的β平面上的奇异涡旋理论大大拓宽了我们对局部地球物理涡旋的演化和动力学的理解,局部地球物理旋涡在海洋和大气的大尺度环流中发挥着重要作用。
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来源期刊
Physical Oceanography
Physical Oceanography OCEANOGRAPHY-
CiteScore
1.80
自引率
25.00%
发文量
8
审稿时长
24 weeks
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