波浪湍流:毛细管波的情况

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Geophysical and Astrophysical Fluid Dynamics Pub Date : 2020-01-28 DOI:10.1080/03091929.2020.1715966
S. Galtier
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引用次数: 2

摘要

毛细管波可能是介绍波浪湍流最简单的例子。自Zakharov和Filonenko发表第一篇论文以来,毛细波湍流一直是许多研究的主题,但仍然缺乏动力学方程的教学推导。本文的目的是在没有重力和深水近似的情况下给出这样的推导。我们使用欧拉方法和围绕平衡高度的速度势的泰勒展开来推导动力学方程。对三波相互作用的定向极性的使用导致了这个方程的紧凑形式,这与以前的工作完全兼容。用所谓的Zakharov变换对波数进行了精确解的推导,并讨论了这些解的性质。本文还回顾了近几十年来所做的实验和数值工作。
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Wave turbulence: the case of capillary waves
ABSTRACT Capillary waves are perhaps the simplest example to consider for an introduction to wave turbulence. Since the first paper by Zakharov and Filonenko, capillary wave turbulence has been the subject of many studies, but a didactic derivation of the kinetic equation is still lacking. It is the objective of this paper to present such a derivation in the absence of gravity and in the approximation of deep water. We use the Eulerian method and a Taylor expansion around the equilibrium elevation for the velocity potential to derive the kinetic equation. The use of directional polarities for three-wave interactions leads to a compact form for this equation which is fully compatible with previous work. The exact solutions are derived with the so-called Zakharov transformation applied to wavenumbers, and the nature of these solutions is discussed. Experimental and numerical works done in recent decades are also reviewed.
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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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