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首页> 外文期刊>Journal of Fluid Mechanics >The critical merger distance between two co-rotating quasi-geostrophic vortices
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The critical merger distance between two co-rotating quasi-geostrophic vortices

机译:两个同向旋转的准地转涡旋之间的临界合并距离

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This paper examines the critical merger or strong interaction distance between two equal-potential-vorticity quasi-geostrophic vortices. The interaction between the two vortices depends on five parameters: their volume ratio, their height-to-width aspect ratios and their vertical and horizontal offsets. Due to the size of the parameter space, a direct investigation solving the full quasi-geostrophic equations is impossible. We instead determine the critical merger distance approximately using an asymptotic approach. We associate the merger distance with the margin of stability for a family of equilibrium states having prescribed aspect and volume ratios, and vertical offset. The equilibrium states are obtained using an asymptotic solution method which models vortices by ellipsoids. The margin itself is determined by a linear stability analysis. We focus on the interaction between oblate to moderately prolate vortices, the shapes most commonly found in turbulence. Here, a new unexpected instability is found and discussed for prolate vortices which is manifested by the tilting of vortices toward each other. It implies than tall vortices may merge starting from greater separation distances than previously thought.
机译:本文研究了两个等势旋涡准地转涡旋之间的临界合并或强相互作用距离。两个漩涡之间的相互作用取决于五个参数:它们的体积比,高度与宽度的纵横比以及它们的垂直和水平偏移。由于参数空间的大小,不可能直接研究求解完整的拟地转方程。相反,我们使用渐近方法近似确定关键合并距离。对于具有规定纵横比和体积比以及垂直偏移的平衡状态族,我们将合并距离与稳定裕度关联起来。使用渐近解法获得平衡态,该渐进解法通过椭圆体对涡旋进行建模。裕度本身是通过线性稳定性分析确定的。我们专注于扁圆形涡和中扁圆形涡之间的相互作用,涡最常见于湍流。在这里,发现并讨论了新的意想不到的不稳定性,这是由于涡旋相互之间的倾斜而表现出来的。这意味着高涡旋可能会比以前认为的更大的分离距离开始合并。

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