在存在表面张力的情况下,柔性底对振荡扰动产生波的影响

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Geophysical and Astrophysical Fluid Dynamics Pub Date : 2023-05-04 DOI:10.1080/03091929.2023.2207018
Selina Hossain, Arijit Das, S. De
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引用次数: 1

摘要

本文研究了有限深度海洋表面时谐压力分布产生波浪的二维问题。在这里,它被认为海洋有一个柔性的基础,它被建模为一个薄的弹性板,并由欧拉-伯努利梁方程控制。还考虑了自由表面表面张力的影响。在水波线性化理论的框架内,利用拉普拉斯-傅立叶变换技术求解了初始边值问题,得到了自由水面高程的积分形式。采用定相法求解大时间、大距离自由面高程的渐近解。不同形式的地表高程以图形形式展示了一些参数的变化,并得出了适当的结论。此外,还利用等值线图推导和分析了与波浪运动相关的频散关系,以了解根的特征。此外,本文还研究了浅水和深水中波浪运动的相速度和群速度。
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The influence of flexible bottom on wave generation by an oscillatory disturbance in the presence of surface tension
The two-dimensional problem of wave generation by a time-harmonic pressure distribution on the surface in a finite-depth ocean is studied in this article. Here, it is considered that the ocean has a flexible base, which is modelled as a thin elastic plate and is governed by the Euler–Bernoulli beam equation. The effect of surface tension at the free surface is also taken into account. Within the framework of the linearised theory of water waves, the initial boundary value problem is solved using the Laplace–Fourier transform technique and the integral form of the free surface elevation is obtained. The method of stationary phase is used to evaluate the asymptotic solutions of the free surface elevation for large time and distance. Different forms of the surface elevation have been demonstrated graphically for variation of parameters in a number of figures, and appropriate conclusions are drawn. Moreover, the dispersion relation associated with the wave motion is also derived and analysed using contour plots to understand the characteristics of the roots. Further, the phase and group velocities of the wave motion have also been investigated in this study for both shallow and deep water.
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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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