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首页> 外文期刊>Journal of Physical Oceanography >Two Different Aperiodic Phases of Wind-Driven Ocean Circulation in a Double-Gyre, Two-Layer Shallow-Water Model
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Two Different Aperiodic Phases of Wind-Driven Ocean Circulation in a Double-Gyre, Two-Layer Shallow-Water Model

机译:双涡流,两层浅水模型中风驱动海洋环流的两个不同的非周期性阶段

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摘要

A two-layer shallow-water model is used to investigate the transition of wind-driven double-gyre circulation from laminar flow to turbulence as the Reynolds number (Re) is systematically increased. Two distinctly different phases of turbulent double-gyre patterns and energy trajectories are exhibited before and after at Re = 95: deterministic and fully developed turbulent circulations. In the former phase, the inertial subgyres vary between an asymmetric solution and an antisymmetric solution and the double-gyre circulations reach the aperiodic solution mainly due to their barotropic instability. An integrated kinetic energy in the lower layer is slight and the generated mesoscale eddies are confined in the upper layer. The power spectrum of energies integrated over the whole domain at Re = 70 has peaks at the interannual periods (4-7 yr) and the interdecadal period (10-20 yr). The loops of the attractors take on one cycle at those periods and display the blue-sky catastrophe. At Re = 95, the double-gyre circulation reaches a metastable state and the attracters obtained from the three energies form a topological manifold. In the latter, as Re increases, the double-gyre varies from a metastable state to a chaotic state because of the barotropic instability of the eastward jet and the baroclinic instability of recirculation retrograde flow, and the eastward jet meanders significantly with interdecadal variability. The generated eddies cascade to the red side of the power spectrum as expected in the geostrophic turbulence. The main results in the simulation may indicate essential mechanisms for the appearance of multiple states of the Kuroshio and for low-frequency variations in the midlatitude ocean.
机译:使用两层浅水模型来研究随着系统雷诺数(Re)的增加,风力驱动的双回旋环流从层流到湍流的过渡。在Re = 95之前和之后,湍流双涡流模式和能量轨迹有两个截然不同的阶段:确定性和充分发展的湍流环流。在前一阶段,惯性子回转体在非对称解和反对称解之间变化,双回转环流达到非周期性解的主要原因是它们的正压不稳定性。在下层中的积分动能很小,并且所产生的中尺度涡流被限制在上层中。在Re = 70时,在整个域中积分的能量的功率谱在年际周期(4-7年)和年代际周期(10-20年)具有峰值。在那个时期,吸引子的循环是一个周期,并显示出蓝天的灾难。在Re = 95时,双回转环流达到亚稳态,从这三种能量获得的吸引子形成拓扑流形。在后者中,随着Re的增加,由于东向射流的正压不稳定性和回流逆流的斜压不稳定性,双旋涡从亚稳态变为混沌状态,并且东向射流的年代际变化显着。正如在地转湍流中所预期的那样,所产生的涡流级联到功率谱的红色侧。模拟的主要结果可能表明黑潮的多种状态的出现和中纬度海洋低频变化的基本机制。

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