首页> 外文期刊>Journal of Geophysical Research, C. Oceans: JGR >Application of an unstructured mesh model to the determination of the baroclinic circulation of the Irish Sea
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Application of an unstructured mesh model to the determination of the baroclinic circulation of the Irish Sea

机译:非结构网格模型在爱尔兰海斜斜环测定中的应用

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摘要

A three‐dimensional finite volume model with horizontally varying, but fixed in time mesh, is used to compute the baroclinic circulation of the Irish Sea during 1995. Tidal forcing was applied along the model’s open boundary with meteorological forcing taken from observations. Initial calculations were performed with a mesh that had high resolution in the well mixed near coastal region; a necessary requirement in order to reproduce tides in the region, although offshore in the stratified area the mesh was slightly coarser than that used in earlier finite difference models. Subsequent calculations were performed using an enhanced resolution which is significantly finer than earlier finite difference models in the offshore region which is thermally stratified in summer due to solar heating and low tidal mixing. This produces a cold water bottom dome separated from the well mixed shallow water regions by strong tidal fronts. Calculations show that both model meshes can reproduce the observed major features of the baroclinic circulation of the western Irish Sea, with the coarse mesh model giving comparable results to earlier finite difference models. In the case of the finer mesh model there are sharper horizontal density gradients in the region of the fronts, which show the presence of baroclinic instability and associated small scale variability as observed in satellite images but not found in the coarser mesh model due to lack of resolution. Results from the fine mesh model show significantly more spatial variability comparable to that found in the measurements.
机译:使用具有水平变化但固定在时间网格中的三维有限体积模型来计算1995年爱尔兰海的斜斜环流。沿该模型的开放边界应用潮汐强迫,并从观测中获取气象强迫。最初的计算是在沿海地区混合良好的高分辨率网格上进行的。尽管在分层区域的近海处,网格比早期的有限差分模型中使用的网格稍粗,但它是在该区域再现潮汐的必要条件。随后的计算使用增强的分辨率进行,该分辨率比海上地区由于太阳能加热和低潮汐混合而在夏季进行热分层的海上有限分层模型要好得多。这样就产生了一个冷水底部穹顶,它与潮汐混合均匀的浅水区域之间被强潮汐前沿隔开。计算表明,两个模型网格都可以重现观察到的西爱尔兰海斜斜环流的主要特征,其中粗网格模型可以提供与早期有限差分模型相当的结果。在较细的网格模型的情况下,在前缘区域存在较尖锐的水平密度梯度,这表明存在斜压不稳定性和相关的小尺度变化,如在卫星图像中观察到的,但由于缺乏网格而在较粗的网格模型中未发现解析度。细网格模型的结果显示,与测量结果相比,空间变异性明显更高。

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