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This book is concerned with the theory of gravity–capillary free-surface flows. Free-surface flows are flows bounded by surfaces that have to be found as part of the solution. A canonical example is that of waves propagating on a water surface, the latter in this case being the free surface.
Many other examples of free-surface flows are considered in the book (cavitating flows, free-surface flows generated by moving disturbances, rising bubbles etc.). I hope to convince the reader of the beauty of such problems and to elucidate some mathematical challenges faced when solving them. Both analytical and numerical methods are presented. Owing to space limitations, some topics could not be covered. These include interfacial flows and the effects of viscosity, compressibility and surfactants. Some further developments of the theories described in the book can be found in the list of references.
Many results presented in the book have grown out of my research over the last 35 years and, of course, out of the research of the whole fluid mechanics community. References to the original papers are given. For this book, I have repeated the older numerical calculations with larger numbers of grid points than was possible at the time. I am pleased to report that the new results are in agreement with the earlier ones!
We now return to the free-surface flow generated by a moving disturbance and extend the results of Chapter 4 to the nonlinear regime. We shall see that the wave trains in the far field (if they exist) are then described by the nonlinear theories of Chapters 5 and 6. Furthermore we will show that the nonuniformities of Figures 4.9 and 4.8 are removed when a nonlinear theory is used. Some nonlinear solutions described in this chapter approach the linear solutions of Chapter 4 as the size of the disturbance approaches zero, while others approach solitary waves.
We have organised the results in the following way. In Section 7.1 we present pure gravity free-surface flows (i.e. g ≠ 0, T = 0) in water of finite depth and show in Section 7.1.1 that the nonuniformity of the linear supercritical solutions near F = 1 (see Figure 4.9) is removed when a nonlinear theory is used. Subcritical flows are considered in Section 7.1.2. In Section 7.2 we consider gravity–capillary free-surface flows. Solutions in water of finite depth are described in Section 7.2.1. We show in Section 7.2.2 that the nonuniformity of the linear theory near α = 0.25 (see Figure 4.8) is removed when a nonlinear theory is used. We examine in Section 7.3 the implications of the existence of multiple branches of periodic gravity–capillary waves (see Sections 5.1.2 and 6.5.3) for free-surface flows generated by moving disturbances in water of infinite depth.
Free-surface problems occur in many aspects of science and everyday life. They can be defined as problems whose mathematical formulation involves surfaces that have to be found as part of the solution. Such surfaces are called free surfaces. Examples of free-surface problems are waves on a beach, bubbles rising in a glass of champagne, melting ice, flows pouring from a container and sails blowing in the wind. In these examples the free surface is the surface of the sea, the interface between the gas and the champagne, the surface of the ice, the boundary of the pouring flow and the surface of the sail.
In this book we concentrate on applications arising in fluid mechanics. We hope to convince the reader of the beauty of such problems and to present the challenges faced when one attempts to describe these flows mathematically. Many of these challenges are resolved in the book but others are still open questions. We will always attempt to present fully nonlinear solutions without restricting assumptions on the smallness of some parameters. Our techniques are often numerical. However, it is the belief of the author that a deep understanding of the structure of the solutions cannot be gained by brute-force numerical approaches. It is crucial to combine numerical methods with analytical techniques, especially when singularities are present.
The first ten chapters of this book were devoted to steady free-surface flows. An equally important topic is that of time-dependent free-surface flows. Boundary integral equation methods can still be used to investigate these problems. The idea is to ‘march in time’ and to solve at each time step a linear integral equation similar to those derived in the previous chapters, by using Cauchy integral equation formula or Green's theorem. Such methods have been developed and used by many authors (see for example and the references cited in these papers). In particular, results have been obtained for breaking waves. An obvious use of time-dependent codes is to study the stability of steady solutions.
In this chapter we will confine our attention to one type of time-dependent free-surface flow, namely gravity–capillary standing waves. We will solve the problem by a series expansion similar to that used in Section 5.1 to study periodic travelling waves. The analysis follows Vanden-Broeck closely. The choice of this problem is motivated by the fact that gravity–capillary standing waves have properties similar to those of Wilton ripples (see Section 6.5.3.1).
We note that a proof of the existence of nonlinear gravity standing waves was provided only recently.
Nonlinear gravity–capillary standing waves
The concept of linear standing waves was introduced in Section 2.4.3. Here we extend the theory of standing waves to the nonlinear regime.
Two fundamental approaches have been used in the previous chapters to calculate free-surface flows. The first involves perturbing known exact solutions. Often these exact solutions are trivial, e.g. a uniform stream. To leading order this approach gives a linear theory (see for example the calculations of Chapter 4) and at higher order a weakly nonlinear theory (see for example the small-amplitude expansions and the Korteweg–de Vries equation of Chapter 5).
In the second approach fully nonlinear solutions are computed. This approach involves a discretisation leading to a system of nonlinear algebraic equations, which is then solved by iteration (e.g. using Newton's method). Iteration requires the choice of an initial guess. These initial guesses are often trivial solutions or asymptotic solutions derived in the first approach. After convergence of the iterations, the solution obtained is then used as an initial guess to compute a new solution for slightly different values of the parameters. For example, the linear solutions of Section 2.4 were used as an initial guess in Chapter 6 to compute a nonlinear solution of small amplitude. This solution was then used as an initial guess to compute a solution of larger amplitude and so on. This method of ‘continuation’ leads to families of solutions; an application is the ‘continuation in ∈’ used in Section 7.1.1. We can then investigate whether other solution branches bifurcate from these branches (see Section 6.5.2.1 for an example).
As shown in the previous chapters, efficient methods for two-dimensional free-surface flows can be derived by using the theory of analytic functions. In particular, free streamline problems, series truncation methods and boundary integral equation methods based on the Cauchy integral formula can be used to obtain highly accurate solutions. Unfortunately such techniques are not available for three-dimensional free-surface flows. However, as we shall see in this chapter, boundary integral equation methods can still be derived using Green's theorem.
Boundary integral equation methods based on Green's theorem can also be used for two-dimensional free-surface flows as an alternative to methods based on the Cauchy integral formula. We first show this for twodimensional free-surface flows generated by moving disturbances in water of infinite depth. Gravity is included in the dynamic boundary condition but surface tension is neglected.
Green's function formulation for two-dimensional problems
We describe the numerical method based on Green's functions by considering the free-surface flows generated by a moving pressure distribution (see Figure 4.4) or by a moving surface-piercing object (see Figure 4.3). We will assume that the water is of infinite depth. The corresponding method based on the Cauchy theorem was described in Chapter 7 for a moving pressure distribution.
Pressure distribution
We consider the two-dimensional free-surface flow generated by a pressure distribution moving at a constant velocity U at the surface of a fluid of infinite depth.
There is a certain body of knowledge and methods that finds application in most branches of fluid mechanics. This book aims to supply a proper theoretical understanding that will permit sensible simplifications to be made in the formulation of problems, and enable the reader to develop analytical models of practical significance. Such analyses can be used to guide more detailed experimental and numerical investigations. As in most technical subjects, such understanding is acquired by detailed study of highly simplified 'model problems'. The first part (Chapters 1-4) is concerned entirely with the incompressible flow of a homogeneous fluid. It was written for the Boston University introductory graduate level course 'Advanced Fluid Mechanics'. The remaining Chapters 5 and 6 deal with dispersive waves and acoustics, and are unashamedly inspired by James Lighthill's masterpiece, Waves in Fluids.
The emergence of observing systems such as acoustically-tracked floats in the deep ocean, and surface drifters navigating by satellite has seen renewed interest in Lagrangian fluid dynamics. Starting from the foundations of elementary kinematics and assuming some familiarity of Eulerian fluid dynamics, this 2006 book reviews the classical and new exact solutions of the Lagrangian framework, and then addresses the general solvability of the resulting general equations of motion. A unified account of turbulent diffusion and dispersion is offered, with applications among others to plankton patchiness in the ocean. Written at graduate level, the book provides the first detailed and comprehensive analytical development of the Lagrangian formulation of fluid dynamics, of interest not only to applied mathematicians but also oceanographers, meteorologists, mechanical engineers, astrophysicists and indeed all investigators of the dynamics of fluids.
The book is an introduction to the branch of fluid mechanics concerned with the production of sound by hydrodynamic flows. It is designed for a one semester introductory course at advanced undergraduate or graduate level. Great care is taken to explain underlying fluid mechanical and acoustic concepts, and to describe as fully as possible the steps in a complicated derivation. The discussion deals specifically with low Mach number flows, which enables the sound produced by 'vortex-surface' interactions to be analysed using the 'compact Green's function'. This provides a routine procedure for estimating the sound, and an easy identification of those parts of a structure that are likely to be important sources of sound. Each chapter ends with a set of problems, many of which can form the basis of an extended student project. The final chapter contains worked examples that have been investigated by students at Boston University.
This book is concerned with partial differential equations applied to fluids problems in science and engineering and is designed for two potential audiences. First, this book can function as a text for a course in mathematical methods in fluid mechanics in non-mathematics departments or in mathematics service courses. The authors have taught both. Second, this book is designed to help provide serious readers of journals (professionals, researchers, and graduate students) in analytical science and engineering with tools to explore and extend the missing steps in an analysis. The topics chosen for the book are those that the authors have found to be of considerable use in their own research careers. These topics are applicable in many areas, such as aeronautics and astronautics; biomechanics; chemical, civil, and mechanical engineering; fluid mechanics; and geophysical flows. Continuum ideas arise in other contexts, and the techniques included have applications there as well.
Large-Eddy Simulations of Turbulence is an ideal introduction for people new to LES [large-eddy simulation], direct numerical simulation and Reynolds-averaged Navier-Stokes simulation, and as a reference for researchers. Of particular interest in the text are the detailed discussion, in Chapter 2, of vorticity, pressure, and the velocity gradient tensor, quantities useful for probing the results of a simulation, particularly when looking for coherent vortices and coherent structures. Chapters 4 and 5 feature an in-depth discussion of spectral subgrid-scale modeling. Although physical-space models are generally more readily applied, spectral models give insight into the requirements and limitations in subgrid-scale modeling and backscattering. A third special feature is the detailed discussion in Chapter 7, of large-eddy simulation of compressible flows previously only available in articles scattered throughout the literature. This will be of interest to those dealing with supersonic flows, combustion, astrophysics, and other related topics.