Wave radiation by a horizontal circular cylinder in a three-layer fluid

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS
Minakshi Ghosh, D. Das
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引用次数: 0

Abstract

To construct cylindrical structures like circular pipe bridges or tunnels submerged in the almost still density-stratified ocean or seawater, the study of waves radiated by the cylinder is essential. This research solves the wave radiation problem by calculating non-dimensionalized added mass and damping coefficients to the mass of the fluid displaced by the submerged horizontal cylinder in either layer of a three-layer fluid, which is still otherwise. Under the linear theory of water waves, we investigate the circular cylinder's hydrodynamic forces by its swaying and heaving motion. The time-harmonic wave propagates with three distinct wavenumbers for a given frequency. The method of multipoles has been employed due to its rapid converging solutions by increasing the truncation limit. Potential functions are expressed into systems of linear algebraic equations, which are solved numerically for two sets of unknowns in each case by truncation. Then, the added mass and damping coefficients are obtained from the non-dimensionalized hydrodynamic forces when the horizontal circular cylinder is submerged in the lower, middle and upper layers, respectively. The obtained results are depicted graphically against wavenumber in numerous figures and analysed.
三层流体中水平圆柱体的波辐射
为了在几乎没有密度分层的海洋或海水中建造像圆形管桥或隧道这样的圆柱形结构,研究圆柱体辐射的波是必不可少的。本研究通过计算三层流体任一层中被淹没水平圆柱体置换的流体质量的无量纲化附加质量和阻尼系数来解决波辐射问题。在水波线性理论的基础上,通过圆柱的摆动和起伏运动研究了圆柱的水动力。在给定频率下,时谐波以三个不同的波数传播。由于多极方法通过增加截断极限而快速收敛,因此采用了多极方法。势函数被表示成线性代数方程组,并通过截断对两组未知量进行数值求解。然后,从无量纲化的水动力中分别得到水平圆柱在下层、中层和上层浸没时的附加质量和阻尼系数。用许多图形将所得结果以波数表示,并进行了分析。
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来源期刊
Geophysical and Astrophysical Fluid Dynamics
Geophysical and Astrophysical Fluid Dynamics 地学天文-地球化学与地球物理
CiteScore
3.10
自引率
0.00%
发文量
14
审稿时长
>12 weeks
期刊介绍: Geophysical and Astrophysical Fluid Dynamics exists for the publication of original research papers and short communications, occasional survey articles and conference reports on the fluid mechanics of the earth and planets, including oceans, atmospheres and interiors, and the fluid mechanics of the sun, stars and other astrophysical objects. In addition, their magnetohydrodynamic behaviours are investigated. Experimental, theoretical and numerical studies of rotating, stratified and convecting fluids of general interest to geophysicists and astrophysicists appear. Properly interpreted observational results are also published.
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