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首页> 外文期刊>Journal of Physical Oceanography >Long Extratropical Planetary Wave Propagation in the Presence of Slowly Varying Mean Flow and Bottom Topography. Part Ⅱ: Ray Propagation and Comparison with Observations
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Long Extratropical Planetary Wave Propagation in the Presence of Slowly Varying Mean Flow and Bottom Topography. Part Ⅱ: Ray Propagation and Comparison with Observations

机译:在缓慢变化的平均流量和底部地形的情况下,长的温带行星行星传播。第二部分:射线传播及其与观测值的比较

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摘要

Ray theory is used to predict phase and group velocities for long planetary waves under realistic, albeit slowly varying, oceanic conditions. The results are compared with local theory using fields smoothed to the same amount (9°latitude/longitude) as well as those with much less smoothing (1°). The agreement is excellent, showing that local theory forms a good proxy for ray theory results. The predicted speeds agree well with observations of planetary waves deduced from sea surface height data. The theory uses purely baroclinic mean flow; the inclusion of barotropic flow has little effect except at high latitudes.
机译:射线理论用于预测在现实的尽管缓慢变化的海洋条件下长行星波的相位和群速度。将结果与局部理论相比较,后者使用平滑到相同量(纬度/经度为9°)和平滑程度较小(1°)的场。该协议非常好,表明局部理论可以很好地替代射线理论的结果。预测的速度与从海面高度数据推导出的行星波观测结果非常吻合。该理论使用纯斜斜平均流量;除在高纬度地区外,正压流的影响很小。

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