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On nonlinear planetary waves: A class of solutions missed by the traditional quasi-geostrophic approximation

机译:在非线性行星波上:传统的准食近似错失的一类解决方案

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Weakly nonlinear quasi-geostrophic planetary waves on a beta-plane and topographic waves over a linearly inclined bottom are examined by use of shallow water equations for a small beta parameter. Long solitary wave solutions missed by the use of the traditional quasi-geostrophic approximation are found in a channel ocean with neither a sheared current nor a curved (non-linearly inclined) bottom topography. The solutions are missed in the traditional approach because the irrotational motion associated with the geostrophic divergence is neglected by the quasi-geostrophic approximation. Another example which calls attention to the limitation of the traditional quasi-geostrophic approximation is the nonlinear evolution of divergent planetary eddies whose scale is much larger than the Rossby's radius of deformation. Some aspects of a new evolution equation are briefly discussed.
机译:通过使用用于小β参数的浅水方程,通过使用浅水方程来检查β面和地形波上的弱非线性准滴度行星波在线性倾斜底部。在沟道海洋中发现了使用传统的准 - 地球节近似错过的长孤立波解决方案,既不是剪切电流也不是弯曲的(非线性倾斜的)底部地形。在传统的方法中错过了解决方案,因为与氨嗜酸性近似忽略了与热性发散相关的无检测运动。另一个呼叫对传统准 - 地球节近似的限制的一个例子是不同行星漩涡的非线性演化,其比例远远大于罗斯比的变形半径。简要讨论了新的演化方程的一些方面。

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