使用普林斯顿海洋模型对濑户内海潮汐进行数值模拟

Q4 Earth and Planetary Sciences
信也 湊
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引用次数: 4

摘要

采用普林斯顿海洋模式(POM)在σ坐标系下对濑户内海的潮汐和风暴潮进行了数值模拟。对于潮汐模拟,我们得到了与天文潮汐相比较好的结果,特别是整体振幅和相位特征。对于风暴潮模拟,模式结果显示的海面高程时间序列与每个站点的观测结果相似。然而,也出现了一些差异。造成这种差异的原因是海面风场覆盖面积大,分辨率不够。然而,在沿海地区风暴潮的重现中,比非线性或三维因素更为重要。使用三维分层模型计算的每个地点的最大海面高程值比使用二维正压模型计算的高10%左右。这里提出了一种物理解释。在我们的模拟中发现潮汐运动和风暴潮几乎是独立的;也就是说,结果仅仅是通过叠加由每个独立作用力驱动的模拟得到的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
プリンストン・オーシャン・モデルを使った, 瀬戸内海の潮汐の数値シミュレーション
Tide and storm surges in the Seto Inland Sea were numerically simulated in a σ-coordinate system using the Princeton Ocean Model (POM). For tide simulation, we obtained good results compared to the astronomical tide, particularly overall amplitude and phase features. For storm surge simulation, results from the model show sea surface elevation time series similar to that observed at each station. Several differences also arise, however. The discrepancy is attributable to the sea surface wind field over a wide area and the lack of sufficient resolution. More important ingredients are involved in reproducing the coastal region storm surge than nonlinearity or 3-dimensionality, however.   Maximum sea surface elevation values for each location calculated using a 3-dimensional, stratified model were found to be up to about 10% larger than those calculated with a 2-dimensional, barotropic model. A physical explanation is proposed here.   Tidal motion and storm surge are found to be almost independent in our simulations; that is, results are obtained merely by superposing the simulation driven by each independent forcing.
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来源期刊
Papers in Meteorology and Geophysics
Papers in Meteorology and Geophysics Earth and Planetary Sciences-Geophysics
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