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  • 1
    facet.materialart.12
    Berlin : Springer
    Call number: 9783662554760 (e-book)
    Description / Table of Contents: This book is the first comprehensive introduction to the theory of equatorially-confined waves and currents in the ocean. Among the topics treated are inertial and shear instabilities, wave generation by coastal reflection, semiannual and annual cycles in the tropic sea, transient equatorial waves, vertically-propagating beams, equatorial Ekman layers, the Yoshida jet model, generation of coastal Kelvin waves from equatorial waves by reflection, Rossby solitary waves, and Kelvin frontogenesis. A series of appendices on midlatitude theories for waves, jets and wave reflections add further material to assist the reader in understanding the differences between the same phenomenon in the equatorial zone versus higher latitudes.
    Type of Medium: 12
    Pages: 1 Online-Ressource (xxiv, 517 Seiten) , Illustrationen
    ISBN: 978-3-662-55476-0 , 9783662554760
    Language: English
    Note: Contents 1 An Observational Overview of the Equatorial Ocean 1.1 The Thermocline: The Tropical Ocean as a Two-Layer Model 1.2 Equatorial Currents 1.3 The Somali Current and the Monsoon 1.4 Deep Internal Jets 1.5 The El Niño/Southern Oscillation (ENSO) 1.6 Upwelling in the Gulf of Guinea 1.7 Seasonal Variations of the Thermocline 1.8 Summary References 2 Basic Equations and Normal Modes 2.1 Model 2.2 Boundary Conditions 2.3 Separation of Variables 2.4 Lamb’s Parameter, Equivalent Depths, Kelvin Phase Speeds and All that 2.5 Vertical Modes and Layer Models 2.6 Nondimensionalization References 3 Kelvin, Yanai, Rossby and Gravity Waves 3.1 Latitudinal Wave Modes: An Overview 3.2 Latitudinal Wave Modes: Structure and Spatial Symmetries 3.3 Dispersion Relations: Exact and Approximate Frequencies 3.4 Analytic Approximations to Equatorial Wave Frequencies 3.4.1 Explicit Formulas 3.4.2 Long Wave Series 3.5 Separation of Time Scales 3.6 Forced Waves 3.7 How the Mixed-Rossby Gravity Wave Earned Its Name 3.8 Hough-Hermite Vector Basis 3.8.1 Introduction 3.8.2 Inner Product and Orthogonality 3.8.3 Orthonormal Basis Functions 3.9 Applications of the Hough-Hermite Basis: Linear Initial-Value Problems 3.10 Initialization Through Hough-Hermite Expansion 3.11 Energy Relationships 3.12 The Equatorial Beta-Plane as the Thin Limit of the Nonlinear Shallow Water Equations on the Sphere References 4 The “Long Wave” Approximation & Geostrophy 4.1 Introduction 4.2 Quasi-Geostrophy 4.3 The “Meridional Geostrophy”, “Low Frequency” or “Long Wave” Approximation 4.4 Boundary Conditions 4.5 Frequency Separation of Slow [Rossby/Kelvin] and Fast [Gravity] Waves 4.6 Initial Value Problems in an Unbounded Ocean, Linearized About a State of Rest, in the Long Wave Approximation 4.7 Reflection from an Eastern Boundary in the Long Wave Approximation 4.7.1 The Method of Images 4.7.2 Dilated Images 4.7.3 Zonal Velocity 4.8 Forced Problems in the Long Wave Approximation References 5 The Equator as Wall: Coastally Trapped Waves and Ray-Tracing 5.1 Introduction 5.2 Coastally-Trapped Waves 5.3 Ray-Tracing For Coastal Waves 5.4 Ray-Tracing on the Equatorial Beta-Plane 5.5 Coastal and Equatorial Kelvin Waves 5.6 Topographic and Rotational Rossby Waves and Potential Vorticity References 6 Reflections and Boundaries 6.1 Introduction 6.2 Reflection of Midlatitude Rossby Waves from a Zonal Boundary 6.3 Reflection of Equatorial Waves from a Western Boundary 6.4 Reflection from an Eastern Boundary 6.5 The Meridional Geostrophy/Long Wave Approximation and Boundaries 6.6 Quasi-normal Modes: Definition and Other Weakly Non-existent Phenomena 6.7 Quasi-normal Modes in the Long Wave Approximation: Derivation 6.8 Quasi-normal Modes in the Long Wave Approximation: Discussion 6.9 High Frequency Quasi-free Equatorial Oscillations 6.10 Scattering and Reflection from Islands References 7 Response of the Equatorial Ocean to Periodic Forcing 7.1 Introduction 7.2 A Hierarchy of Models for Time-Periodic Forcing 7.3 Description of the Model and the Problem 7.4 Numerical Models: Reflections and “Ringing” 7.5 Atlantic Versus Pacific 7.6 Summary References 8 Impulsive Forcing and Spin-Up 8.1 Introduction 8.2 The Reflection of the Switched-On Kelvin Wave 8.3 Spin-Up of a Zonally-Bounded Ocean: Overview 8.4 The Interior (Yoshida) Solution 8.5 Inertial-Gravity Waves 8.6 Western Boundary Response 8.7 Sverdrup Flow on the Equatorial Beta-Plane 8.8 Spin-Up: General Considerations 8.9 Equatorial Spin-Up: Details 8.10 Equatorial Spin-Up: Summary References 9 Yoshida Jet and Theories of the Undercurrent 9.1 Introduction 9.2 Wind-Driven Circulation in an Unbounded Ocean: f-Plane 9.3 The Yoshida Jet 9.4 An Interlude: Solving Inhomogeneous Differential Equations at Low Latitudes 9.4.1 Forced Eigenoperators: Hermite Series 9.4.2 Hutton–Euler Acceleration of Slowly Converging Hermite Series 9.4.3 Regularized Forcing 9.4.4 Bessel Function Explicit Solution for the Yoshida Jet 9.4.5 Rational Approximations: Two-Point Padé Approximants and Rational Chebyshev Galerkin Methods 9.5 Unstratified Models of the Undercurrent 9.5.1 Theory of Fofonoff and Montgomery (1955) 9.5.2 Model of Stommel (1960) 9.5.3 Gill (1971) and Hidaka (1961) References 10 Stratified Models of Mean Currents 10.1 Introduction 10.2 Modal Decompositions for Linear, Stratified Flow 10.3 Different Balances of Forces 10.3.1 Bjerknes Balance 10.4 Forced Baroclinic Flow in the “Bjerknes” Approximation 10.4.1 Other Balances 10.5 The Sensitivity of the Undercurrent to Parameters 10.6 Observations of Subsurface Countercurrents (Tsuchiya Jets) 10.7 Alternate Methods for Vertical Structure with Viscosity 10.8 McPhaden’s Model of the EUC and SSCC’s: Results 10.9 A Critique of Linear Models of the Continuously-Stratified, Wind-Driven Ocean References 11 Waves and Beams in the Continuously Stratified Ocean 11.1 Introduction 11.1.1 Equatorial Beams: A Theoretical Inevitability 11.1.2 Slinky Physics and Impedance Mismatch, or How Water Can Be as Reflective as Silvered Glass 11.1.3 Shallow Barriers to Downward Beams 11.1.4 Equatorial Methodology 11.2 Alternate Form of the Vertical Structure Equation 11.3 The Thermocline as a Mirror 11.4 The Mirror-Thermocline Concept: A Critique 11.5 The Zonal Wavenumber Condition for Strong Excitation of a Mode 11.6 Kelvin Beams: Background 11.7 Equatorial Kelvin Beams: Results References 12 Stable Linearized Waves in a Shear Flow 12.1 Introduction 12.2 UðyÞ: Pure Latitudinal Shear 12.3 Neutral Waves in Flow Varying with Both Latitude and Height: Numerical Studies 12.4 Vertical Shear and the Method of Multiple Scales References 13 Inertial Instability, Pancakes and Deep Internal Jets 13.1 Introduction: Stratospheric Pancakes and Equatorial Deep Jets 13.2 Particle Argument 13.2.1 Linear Inertial Instability 13.3 Centrifugal Instability: Rayleigh’s Parcel Argument 13.4 Equatorial Gamma-Plane Approximation 13.5 Dynamical Equator 13.6 Gamma-Plane Instability 13.7 Mixed Kelvin-Inertial Instability 13.8 Summary References 14 Kelvin Wave Instability: Critical Latitudes and Exponentially Small Effects 14.1 Proxies and the Optical Theorem 14.2 Six Ways to Calculate Kelvin Instability 14.2.1 Power Series for the Eigenvalue 14.2.2 Hermite-Padé Approximants 14.2.3 Numerical Methods 14.3 Instability for the Equatorial Kelvin Wave in the Small Wavenumber Limit 14.3.1 Beyond-All-Orders Rossby Wave Instability 14.3.2 Beyond-All-Orders Kelvin Wave Instability in Weak Shear in the Long Wave Approximation 14.4 Kelvin Instability in Shear: The General Case References 15 Nonmodal Instability 15.1 Introduction 15.2 Couette and Poiseuille Flow and Subcritical Bifurcation 15.3 The Fundamental Orr Solution 15.4 Interpretation: The “Venetian Blind Effect” 15.5 Refinements to the Orr Solution 15.6 The “Checkerboard” and Bessel Solution 15.6.1 The “Checkerboard” Solution 15.7 The Dandelion Strategy 15.8 Three-Dimensional Transients 15.9 ODE Models and Nonnormal Matrices 15.10 Nonmodal Instability in the Tropics 15.11 Summary References 16 Nonlinear Equatorial Waves 16.1 Introduction 16.2 Weakly Nonlinear Multiple Scale Perturbation Theory 16.2.1 Reduction from Three Space Dimensions to One 16.2.2 Three Dimensions and Baroclinic Modes 16.3 Solitary and Cnoidal Waves 16.4 Dispersion and Waves 16.4.1 Derivation of the Group Velocity Through the Method of Multiple Scales 16.5 Integrability, Chaos and the Inverse Scattering Method 16.6 Low Order Spectral Truncation (LOST) 16.7 Nonlinear Equatorial Kelvin Waves 16.7.1 Physics of the One-Dimensional Advection (ODA) Equation: ut + cux + buux = 0 16.7.2 Post-Breaking: Overturning, Taylor Shock or “Soliton Clusters”? 16.7.3 Viscous Regularization of Kelvin Fronts: Burgers’ Equation And Matched Asymptotic Perturbation Theory 16.8 Kelvin-Gravity Wave Shortwave Resonance: Curving Fronts and Undulations 16.9 Kelvin Solitary and Cnoidal Waves 16.10 Corner Waves and the Cnoidal-Corner-Breaking Scenario 16.11 Rossby Solitary Waves 16.12 Antisymmetr
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  • 2
    Electronic Resource
    Electronic Resource
    New York, NY : American Institute of Physics (AIP)
    Physics of Fluids 4 (1992), S. 2578-2581 
    ISSN: 1089-7666
    Source: AIP Digital Archive
    Topics: Physics
    Notes: Critical parameters (Reynolds number and wave number) signaling the onset of Taylor vortices are calculated for the flow between "elliptical'' cylinders. The spinning inner cylinder is circular; the stationary outer cylinder is composed of two circular arcs and is similar to an ellipse. It is shown that increasing ellipticity destabilizes the flow and increasing eccentricity stabilizes the flow. The spectral element method is used to calculate the base flow and to solve the linear stability problem.
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  • 3
    Electronic Resource
    Electronic Resource
    Springer
    Acta applicandae mathematicae 56 (1999), S. 1-98 
    ISSN: 1572-9036
    Keywords: perturbation methods ; asymptotic ; hyperasymptotic ; exponential smallness
    Source: Springer Online Journal Archives 1860-2000
    Topics: Mathematics
    Notes: Abstract Singular perturbation methods, such as the method of multiple scales and the method of matched asymptotic expansions, give series in a small parameter ε which are asymptotic but (usually) divergent. In this survey, we use a plethora of examples to illustrate the cause of the divergence, and explain how this knowledge can be exploited to generate a 'hyperasymptotic' approximation. This adds a second asymptotic expansion, with different scaling assumptions about the size of various terms in the problem, to achieve a minimum error much smaller than the best possible with the original asymptotic series. (This rescale-and-add process can be repeated further.) Weakly nonlocal solitary waves are used as an illustration.
    Type of Medium: Electronic Resource
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  • 4
    Electronic Resource
    Electronic Resource
    Springer
    Zeitschrift für angewandte Mathematik und Physik 40 (1989), S. 940-944 
    ISSN: 1420-9039
    Source: Springer Online Journal Archives 1860-2000
    Topics: Mathematics , Physics
    Notes: Abstract Toda [1], Boyd [2], Zaitsev [3], Korpel & Banerjee [4], and Whitham [5] have proved that many species of solitons may be cloned and superposed with even spacing to generateexact nonlinear, spatially periodic solutions (“cnoidal waves”). The equations solved by such “imbricate” series of solitary waves include the Korteweg-deVries, Cubic Schroedinger, Benjamin-Ono, and resonant triad equations. However, all existing theorems apply only when the solitons arerational ormeromorphic functions and the cnoidal waves areelliptic functions. In this note, we ask: does the exact soliton-superposition apply to non-elliptic solitons and cnoidal waves? Although a complete answer to this (very broad!) question eludes us, it is possible to offer a revealing counterexample. The quartic Korteweg-deVries equation has solutions which arehyperelliptic, and thus very special. Nevertheless, its periodic solutions are not the exact superposition of the infinite number of copies of a soliton. This is highly suggestive that non-elliptic extensions of the Toda theorem are rare or non-existent. It is intriguing, however, that the soliton-superposition generates a very goodapproximation to the hypercnoidal wave even when the solitons strongly overlap.
    Type of Medium: Electronic Resource
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  • 5
    ISSN: 1573-7691
    Keywords: Hyperviscous ; shocks ; diffusion ; shock capturing
    Source: Springer Online Journal Archives 1860-2000
    Topics: Computer Science
    Notes: Abstract We solve two problems ofx∈[−∞, ∞] for arbitrary orderj. The first is to compute shock-like solutions to the hyperdiffusion equation,u1=(−1) j+1 u 2j,x. The second is to compute similar solutions to the stationary form of the hyper-Burgers equation, (−1) j u 2j.x+uu x=0; these tanh-like solutions are asymptotic approximations to the shocks of the corresponding time dependent equation. We solve the hyperdiffusion equation with a Fourier integral and the method of steepest descents. The hyper Burgers equation is solved by a Fourier pseudospectral method with a polynomial subtraction. Except for the special case of ordinary diffusion (j=1), the jump across the shock zone is described bynonmonotonic, oscillatory functions. By smearing the front over the width of a grid spacing, it is possible to numerically resolve the shock with a weaker and weaker viscosity coefficient asj, the order of the damping, increases. This makes such “hyperviscous” dampings very attractive for coping with fronts since, outside the frontal zone, the impact of the artificial hyperviscosity is much smaller than with ordinary viscosity. Unfortunately, both the intensity of the oscillations and the slowness of their exponential decay from the center of the shock zone decrease asj increases so that the shock zone is muchwider than for ordinary diffusion. We also examined generalizations of Burgers equation with “spectral viscosity”, that is, damping which is tailored to yield exponentially small errors outside the frontal zone when combined with spectral methods. We find behavior similar to high order hyperviscosity. We conclude that high order damping, as a tool for shock-capturing, offers both advantages and drawbacks. Monotonicity, which has been the holy grail of so much recent algorithm development, is a reasonable goal only for ordinary viscosity. Hyperviscous fronts and shock zones in flows with “spectral viscosity” aresupposed to oscillate.
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  • 6
    Electronic Resource
    Electronic Resource
    Springer
    Journal of scientific computing 5 (1990), S. 311-363 
    ISSN: 1573-7691
    Keywords: Interpolation error ; Fourier method ; Chebyshev method ; pseudospectral method
    Source: Springer Online Journal Archives 1860-2000
    Topics: Computer Science
    Notes: Abstract The error in Chebyshev or Fourier interpolation is the product of a rapidly varying factor with a slowly varying modulation. This modulation is the “envelope” of the error. Because this slow modulation controls the amplitude of the error, it is crucial to understand this “error envelope.” In this article, we show that the envelope varies strongly withx, but its variations can be predicted from the convergence-limiting singularities of the interpolated function f(x). In turn, this knowledge can be translated into a simple spectral correction algorithm for wringing more accuracy out of the same pseudospectral calculation of the solution to a differential equation.
    Type of Medium: Electronic Resource
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  • 7
    Electronic Resource
    Electronic Resource
    Springer
    Journal of scientific computing 2 (1987), S. 99-109 
    ISSN: 1573-7691
    Keywords: Quadrature ; rational Chebyshev functions ; adaptive quadrature ; numerical integration
    Source: Springer Online Journal Archives 1860-2000
    Topics: Computer Science
    Notes: Abstract The Clenshaw-Curtis method for numerical integration is extended to semi-infinite ([0, ∞] and infinite [-∞, ∞] intervals. The common framework for both these extensions and for integration on a finite interval is to (1) map the integration domain tol ε [0,π], (2) compute a Fourier sine or cosine approximation to the transformd integrand via interpolation, and (3) integrate the approximation. The interpolation is most easily performed via the sine or cosine cardinal functions, which are discussed in the appendix. The algorithm is mathematically equivalent to expanding the integrand in (mapped or unmapped) Chebyshev polynomials as done by Clenshaw and Curtis, but the trigonometric approach simplifies the mechanics. Like Gaussian quadrature, the error for the change-of-coordinates Fourier method decreases exponentially withN, the number of grid points, but the generalized Curtis-Clenshaw algorithm is much easier to program than Gaussian quadrature because the abscissas and weights are given by simple, explicit formulas.
    Type of Medium: Electronic Resource
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  • 8
    Electronic Resource
    Electronic Resource
    Springer
    Journal of scientific computing 3 (1988), S. 109-120 
    ISSN: 1573-7691
    Keywords: Spectral methods ; Fourier series ; Chebyshev polynomials
    Source: Springer Online Journal Archives 1860-2000
    Topics: Computer Science
    Notes: Abstract “Domain truncation” is the simple strategy of solving problems onyε [-∞, ∞] by using a large but finite computational interval, [− L, L] Sinceu(y) is not a periodic function, spectral methods have usually employed a basis of Chebyshev polynomials,T n(y/L). In this note, we show that becauseu(±L) must be very, very small if domain truncation is to succeed, it is always more efficient to apply a Fourier expansion instead. Roughly speaking, it requires about 100 Chebyshev polynomials to achieve the same accuracy as 64 Fourier terms. The Fourier expansion of a rapidly decaying but nonperiodic function on a large interval is also a dramatic illustration of the care that is necessary in applying asymptotic coefficient analysis. The behavior of the Fourier coefficients in the limitn→∞ for fixed intervalL isnever relevant or significant in this application.
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  • 9
    Electronic Resource
    Electronic Resource
    Springer
    Journal of scientific computing 1 (1986), S. 183-206 
    ISSN: 1573-7691
    Keywords: Bratu's problem ; nonlinear eigenvalue problem ; spectral methods
    Source: Springer Online Journal Archives 1860-2000
    Topics: Computer Science
    Notes: Abstract Bratu's problem, which is the nonlinear eigenvalue equationΔu+λ exp(u)=0 withu=0 on the walls of the unit square andλ as the eigenvalue, is used to develop several themes on applications of Chebyshev pseudospectral methods. The first is the importance ofsymmetry: because of invariance under the C4 rotation group and parity in bothx andy, one can slash the size of the basis set by a factor of eight and reduce the CPU time by three orders of magnitude. Second, the pseudospectral method is ananalytical as well as a numerical tool: the simple approximationλ≈3.2A exp(−0.64A), whereA is the maximum value ofu(x, y), is derived via collocation with but a single interpolation point, but is quantitatively accurate for small and moderateA. Third, the Newton-Kantorovich/Chebyshev pseudospectral algorithm is so efficient that it is possible to compute good numerical solutions—five decimal places—on amicrocomputer inbasic. Fourth, asymptotic estimates of the Chebyshev coefficients can be very misleading: the coefficients for moderately or strongly nonlinear solutions to Bratu's equations fall off exponentially rather than algebraically withv untilv is so large that one has already obtained several decimal places of accuracy. The corner singularities, which dominate the behavior of the Chebyshev coefficients in thelimit v→∞, are so weak as to be irrelevant, and replacing Bratu's problem by a more complicated and realistic equation would merely exaggerate the unimportance of the corner branch points even more.
    Type of Medium: Electronic Resource
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  • 10
    Electronic Resource
    Electronic Resource
    Chichester : Wiley-Blackwell
    International Journal for Numerical Methods in Fluids 20 (1995), S. 393-414 
    ISSN: 0271-2091
    Keywords: shallow water equations ; spectral element ; implicit scheme ; GMRES solver ; staggered mesh ; North Atlantic ; Engineering ; Engineering General
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Mechanical Engineering, Materials Science, Production Engineering, Mining and Metallurgy, Traffic Engineering, Precision Mechanics
    Notes: A staggered spectral element model for the solution of the oceanic shallow water equations is presented. We introduce and compare both an implicit and an explicit time integration scheme. The former splits the equations with the operator-integration factor method and solves the resulting algebraic system with generalized minimum residual (GMRES) iterations. Comparison of the two schemes shows the performance of the implicit scheme to lag that of the explicit scheme because of the unpreconditioned implementation of GMRES. The explicit code is successfully applied to various geophysical flows in idealized and realistic basins, notably to the wind-driven circulation in the North Atlantic Ocean. The last experiment reveals the geometric versatility of the spectral element method and the effectiveness of the staggering in eliminating sprious pressure modes when the flow is nearly non-divergent.
    Additional Material: 12 Ill.
    Type of Medium: Electronic Resource
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