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Wind-driven ocean circulation transition to barotropic instability
Authors:Christian Le Provost  Jacques Verron
Affiliation:1. I.M.A.T.I - CNR, Pavia, Italy;2. Dipartimento di Scienze Matematiche, Politecnico di Torino, Italy;1. Graduate School of Informatics, Kyoto University, Kyoto 606-8501, Japan;2. Graduate School of Engineering, Kyoto University, Kyoto 615-8540, Japan;1. School of Mathematics and Information Engineering, Chongqing University of Education, Chongqing 400065, PR China;2. School of Mathematical Sciences, Chongqing Normal University, Chongqing 400047, PR China;3. Key Laboratory for Optimization and Control Ministry of Education, Chongqing Normal University, Chongqing 400047, PR China;1. College of Mathematics and Statistics, Changsha University of Science and Technology, Changsha 410114, China;2. Hunan Provincial Key Laboratory of Mathematical Modeling and Analysis in Engineering, Changsha 410114, China;3. LSEC, Academy of Mathematics and Systems Science, Chinese Academy of Sciences, Beijing 100190, China;4. School of Science, East China Jiaotong University, Nanchang 330013, China
Abstract:This article deals with the ocean circulation driven by steady zonal winds, and damped by bottom and biharmonic friction, when represented by the simple barotropic vorticity equation. A double gyre antisymmetrical wind stress pattern in a square basin is considered. Wind forcing and dissipation parameters are chosen within the ranges of what has been used in previous studies. The flow characteristics for both steady and unsteady situations are tentatively described as functions of model external parameters through the analysis of a large set of numerical experiments. Functional relations are derived for the mid-latitude jet parameters (length, width and transport) on the basis of scaling arguments. With the diagrams established for these quantities in forcing and dissipation parameter relations allow quantitative predictions of model response to a wide range of parameter choices to be made. The transition to barotropic instability is interpreted by analysing and comparing the spin-up phase of different numerical experiments leading either to stable or unstable solutions. Two major types of destabilization are identified, namely through meandering of the mid-latitude eastward jet and Rossby wave radiation from the westward return flow. The characteristics of the flows are shown to be highly sensitive to the external parameter changes. Competition between eddy kinetic energy level and eastward jet extension appears to consttitute the key point of this class of solutions, controlling in particular the intensity of transport in the inner gyres, driven by the eddy field on the two sides of the mid-basin jet, in a very similar manner to that of the more complex multilayered EGCMs.
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