任意海床上厚垂直屏障对波浪散射的耦合特征函数展开-边界元法

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS
A. Choudhary, S. Koley, S. C. Martha
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引用次数: 4

摘要

分析了任意海床上具有厚垂直屏障的波浪结构相互作用问题。采用特征函数展开-边界元耦合方法处理了相应的边值问题。该方法将边值问题转化为物理边界上的积分方程。物理边界被离散成有限数量的元素,因此积分方程产生线性代数方程组。最后对方程组进行求解,得到物理量,即反射系数和透射系数。为了保证这些物理量的正确性,推导并验证了能量平衡关系。通过比较文献中的结果,也验证了目前的结果。研究表明,结构体的宽度和高度与起伏的海底结构在构筑有效的波浪屏障以保护各种海洋设施免受波浪攻击方面发挥着重要作用,同时也有助于在结构体背风侧形成宁静区。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Coupled eigenfunction expansion–boundary element method for wave scattering by thick vertical barrier over an arbitrary seabed
Wave structure interaction problem having thick vertical barrier over an arbitrary seabed is analysed for its solution. The associated boundary value problem is handled using a coupled eigenfunction expansion–boundary element method. This method converts the boundary value problem into integral equation over the physical boundaries. The physical boundaries are discretised into a finite number of elements and hence the integral equation give rise to a system of linear algebraic equations. Finally, the system of equations is solved to obtain the physical quantities, namely, the reflection and transmission coefficients. For ensuring the correctness of these physical quantities, the energy balance relation is derived and verified. The present results are also verified by comparing the results available in the literature. The present study reveals that the width and height of the structure along with the undulated seabed play an important role to construct an effective wave barrier to protect various marine facilities from wave attack and also helpful to create the tranquility zone on the lee side of the structure.
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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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