Numerical simulation of Rossby wave in shallow water

被引:7
|
作者
Sun, Wen-Yih [1 ,2 ,3 ]
Sun, Oliver M. [4 ]
机构
[1] Purdue Univ, Dept Earth Atmospher & Planetary Sci, W Lafayette, IN 47907 USA
[2] Natl Cent Univ, Dept Atmospher Sci, Tao Yuan 320, Taiwan
[3] Nagoya Univ, Hydrospher Atmospher Res Ctr HyARC, Nagoya, Aichi 4648601, Japan
[4] Woods Hole Oceanog Inst, Dept Phys Oceanog, Woods Hole, MA 02543 USA
关键词
Rossby wave; Equatorial beta-plane; Semi-implicit finite volume; Semi-Largangian scheme; LAGRANGIAN ADVECTION SCHEME; EQUATORIAL SOLITARY WAVES; FLOWS; EQUATIONS;
D O I
10.1016/j.compfluid.2013.01.018
中图分类号
TP39 [计算机的应用];
学科分类号
081203 ; 0835 ;
摘要
The semi-implicit, finite volume scheme developed by Sun [13] has been applied to simulate the Rossby waves in the equatorial beta-plane discussed by Boyd [1,2]. The scheme is simple and flexible, and more accurate than the finite volume, flux-form semi-Lagrangian, Lax-Wendroff scheme, and the others presented in Chu and Fan [3]. Compared with the analytic solution, the scheme with the quadratic upstream interpolation for convective kinetics and Shuman smoothing produces less dispersion than that using the 4th-order advection without smoothing. The results also confirm the perturbation theory that predicts solitary waves of large amplitude containing a region of recirculating fluid trapped within the moving disturbance. The general patterns simulated from the initial zeroth-order solutions and the sum of the zeroth-and first-order solutions remain very similar, although the detail and propagation speed can be different. (C) 2013 Elsevier Ltd. All rights reserved.
引用
收藏
页码:116 / 127
页数:12
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