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首页> 外文期刊>Journal of Fluid Mechanics >Meridional dynamics of grounded abyssal water masses on a sloping bottom in a mid-latitude beta-plane
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Meridional dynamics of grounded abyssal water masses on a sloping bottom in a mid-latitude beta-plane

机译:中纬度β面倾斜底部倾斜底部地下深层水群的子午线

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Observations, numerical simulations and theoretical scaling arguments suggest that in mid-latitudes, away from the source regions and the equator, the meridional transport of abyssal water masses along a continental slope corresponds to planetary geostrophic flows that are gravity- or density-driven and topographically steered. We investigate these dynamics using a nonlinear reduced-gravity model that can describe grounded abyssal meridional flow over sloping topography that crosses the planetary vorticity gradient. Exact nonlinear steady and time-dependent solutions are obtained. The general steady theory is illustrated for a non-parallel equatorward flow that possesses a single along-slope grounding along the upslope flank of the current (complementing previous work). Four specific nonlinear time-dependent solutions are described. Two initial-value problems are solved exactly. The first initial configuration corresponds to an equatorward abyssal flow that has no cross-slope shear in the along-slope velocity and possesses a single grounding along the upslope flank of the current. The nonlinear time-dependent evolution of this initial current into a non-parallel shear flow is described. The second initial condition corresponds to an isolated radially symmetric grounded abyssal pool or dome. The nonlinear time-dependent evolution of this abyssal dome, which propagates equatorward with unsteady along- and cross-slope velocities while deforming into an elliptically shaped abyssal dome with beta-induced diminishing height, is described. Finally, the nonlinear time-dependent boundary-value problem can be solved exactly in which the in-flow boundary condition on the poleward boundary of the mid-latitude domain corresponds to a time-dependent abyssal current with both an upslope and downslope grounding. Two specific time-dependent boundary conditions are examined. The first corresponds to a time-limited surge in the equatorward volume transport in the abyssal current along
机译:观察,数值模拟和理论缩放争论表明,在中纬度地区,远离源区和赤道,沿大陆坡度的深度水块的子宫内传输对应于行星出脱节流,这些流量是重力或密度驱动和地拓扑的转向。我们使用非线性减小重力模型来研究这些动态,该模型可以描述接地的深层化学流量,这些流出倾斜的地形,其穿过行星涡度梯度。获得精确的非线性稳态和时间依赖性解决方案。通过沿着电流上的上升侧的侧面(补充以前的工作)具有单个沿斜率接地的非平行赤道流程来说明一般稳定理论。描述了四个特定的非线性时间依赖性解决方案。完全解决了两个初始值问题。第一初始配置对应于赤道的深度流动,其在沿着斜率速度下没有横斜剪切并且具有沿电流的上盖侧的单个接地。描述了该初始电流在非平行剪切流中的非线性时间依赖性演化。第二个初始条件对应于隔离径向对称的自动池或圆顶。描述了这种深度圆顶的非线性时间依赖性演化,其在与β诱导的缩小高度变形的同时使逆转速度和横向速度变形在椭圆形的深度圆顶的同时。最后,可以完全解决非线性时间依赖性边值问题,其中中纬度域的极向边界上的流动边界条件对应于具有上升和下坡接地的时间依赖的深度电流。检查了两个特定的时间依赖边界条件。首先对应于赤道电流中的赤道体积传输中的时间限制浪涌

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