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首页> 外文期刊>Journal of Physical Oceanography >Effects of Mean Flow Direction on Energy, Isotropy, and Coherence of Baroclinically Unstable Beta-Plane Geostrophic Turbulence
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Effects of Mean Flow Direction on Energy, Isotropy, and Coherence of Baroclinically Unstable Beta-Plane Geostrophic Turbulence

机译:平均流向对斜压不稳定β平面地转湍流能量,各向同性和相干性的影响

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The effects of mean flow direction on statistically steady, baroclinically unstable, beta-plane quasigeostrophic (QG) turbulence are examined in a two-layer numerical model. The turbulence is forced by an imposed, horizontally homogeneous, vertically sheared mean flow and dissipated by bottom Ekman friction. The model is meant to be an idealization of the midocean eddy field, which generally has kinetic energies larger than the mean and is isotropic. Energetic eddies can be generated even when planetary beta (β) dominates gradients of mean potential vorticity (PV; also, q), as long as the mean shear has a substantial meridional component. However, eddies are isotropic only when the angle between layer mean PV gradients exceeds approximately 90°. This occurs when planetary and shear-induced gradients are comparable. Maps of PV indicate that these gradients may indeed be comparable over much of the midocean. Coherent jets form when the mean flow has a substantial meridional component and β is large. When β is nonzero, but small enough to permit isotropy, and the zonal component of the mean flow is not strongly eastward, lattices of like-signed coherent vortices develop. Like-signed vortex formation from initial and forcing conditions without a vorticity preference has not been observed before in QG systems. The vortex arrays are sensitive to the details of small-scale dissipation. Both cyclonic and anticyclonic fields arise in the simulations, depending on initial conditions, but they have different energies, consistent with broken symmetries in the governing equations.
机译:在两层数值模型中检查了平均流向对统计稳定,斜压不稳定,β平面拟营养(QG)湍流的影响。湍流由施加的水平均质,垂直剪切的平均流推动,并通过底部埃克曼摩擦消散。该模型是对中洋涡流场的理想化,该涡流场通常具有比均值大的动能并且是各向同性的。即使平均β(β)在平均潜在涡度(PV;也为q)的梯度中占主导地位,也可以生成高能涡流,只要平均切变具有实质的子午分量即可。但是,仅当层平均PV梯度之间的角度超过大约90°时,涡流才是各向同性的。当行星梯度和切变引起的梯度可比较时,就会发生这种情况。 PV的图表明,这些梯度在中洋大部分地区可能确实是可比的。当平均流具有重要的子午分量并且β大时,会形成相干射流。当β非零,但足够小以允许各向同性,并且平均流的纬向分量不强烈向东时,会形成具有相似符号的相干涡旋的晶格。在QG系统中,从未观察到由初始条件和强迫条件形成的类似符号的旋涡,没有旋涡偏好。涡流阵列对小规模耗散的细节很敏感。取决于初始条件,模拟中会出现气旋和反气旋场,但它们具有不同的能量,这与控制方程式中的对称性破坏一致。

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