在理想的海底地形上分析海底摩擦对浅水波浪的影响

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Geophysical and Astrophysical Fluid Dynamics Pub Date : 2023-03-04 DOI:10.1080/03091929.2023.2204430
Chang Liu, A. Clark
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引用次数: 0

摘要

分析海底摩擦对海底地形上浅水波浪的影响在环境和海岸工程以及海洋和大气科学等领域都很重要。然而,目前的理论发展依赖于对这些流动做出某些限制性假设,因此需要更多的发展来进一步概括这种行为。这项工作使用Adomian分解方法(ADM)不仅开发了描述这种行为的半解析公式,对于平坦的地形,而且还作为逆向工程机制开发了描述这种现象的新的封闭形式的解决方案。具体来说,我们分别关注了有限逃逸时间的惯性地转振荡和反气旋涡,我们的结果直接证明了恒定的科里奥利力、恒定的底部摩擦和整体动力学之间的直接关系。此外,我们还说明了在这些类型的流动中,相对于恒定的底部摩擦,耗散引起的不稳定性的要素,在某些情况下,我们还展示了与初始动力学的联系。
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Analysing the impact of bottom friction on shallow water waves over idealised bottom topographies
Analysing the impact of bottom friction on shallow water waves over bottom terrains is important in areas including environmental and coastal engineering as well as the oceanic and atmospheric sciences. However, current theoretical developments rely on making certain limiting assumptions about these flows and thus more development is needed to be able to further generalise this behaviour. This work uses Adomian decomposition method (ADM) to not only develop semi-analytical formulations describing this behaviour, for flat terrains, but also as reverse-engineering mechanisms to develop new closed-form solutions describing this type of phenomena. Specifically, we respectively focus on inertial geostrophic oscillations and anticyclonic vortices with finite escape times in which our results directly demonstrate the direct correlation between the constant Coriolis force, the constant bottom friction, and the overall dynamics. Additionally, we illustrate elements of dissipation-induced instability with respect to constant bottom friction in these types of flows where we also demonstrate the connection to the initial dynamics for certain cases.
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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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