Topographically generated eddies

Herbert E. Huppert , Kirk Bryan
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引用次数: 208

Abstract

The interaction between temporally varying currents and the bottom topography of the ocean is investigated by the numerical and analytic examination of the following simple model. The flow of an inviscid, stratified fluid is initiated from relative rest in a uniformly rotating system containing an isolated topographic feature. The evolution of the flow redistributes vorticity and temperature in such a way that relatively cold water with anticyclonic vorticity exists over the topographic feature, while water shed from above the topographic feature sinks, thereby inducing a warm anomaly with cyclonic vorticity. For sufficiently strong oncoming flows, the shed fluid continually drifts downstream in the form of a relatively warm eddy. If the oncoming flow is relatively weak, the interaction between the anticyclonic and cyclonic vorticity distributions traps the warm eddy and it remains in the vicinity of the topographic feature.

We suggest that recent observations of an eddy in the vicinity of the Atlantis II Seamount and the existence of the large amount of high frequency energy near the bottom of the ocean measured by the MODE experiment may be partly explained in terms of the above mechanism. We conclude by speculating that vorticity redistribution by topography may be a contributing factor to cyclogenesis in the atmosphere.

地形上产生的涡流
通过以下简单模型的数值和解析检验,研究了时变洋流与海底地形之间的相互作用。一种无粘性的分层流体的流动是从一个包含孤立地形特征的均匀旋转系统中的相对静止开始的。气流的演化使涡度和温度重新分布,在地形特征上方存在相对较冷的反气旋涡度水体,而地形特征上方的降水下沉,从而引起气旋涡度温暖异常。对于足够强的迎面而来的气流,脱落的流体以相对温暖的涡流的形式不断向下游漂移。如果迎面而来的气流相对较弱,反气旋和气旋涡度分布之间的相互作用将困住暖涡并使其停留在地形特征附近。我们认为,最近在亚特兰蒂斯II号海山附近观测到的涡旋和MODE实验测量到的海底附近大量高频能量的存在可能部分地解释了上述机制。我们推测地形引起的涡度再分布可能是大气中气旋形成的一个促成因素。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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