Geometric Lagrangian Averaged Euler-Boussinesq and Primitive Equations 2
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Variational Formulation of Fluid and Geophysical Fluid Dynamics
Advances in Geophysical and Environmental Mechanics and Mathematics Gualtiero Badin Fulvio Crisciani Variational Formulation of Fluid and Geophysical Fluid Dynamics Mechanics, Symmetries and Conservation Laws Advances in Geophysical and Environmental Mechanics and Mathematics Series editor Holger Steeb, Institute of Applied Mechanics (CE), University of Stuttgart, Stuttgart, Germany More information about this series at http://www.springer.com/series/7540 Gualtiero Badin • Fulvio Crisciani Variational Formulation of Fluid and Geophysical Fluid Dynamics Mechanics, Symmetries and Conservation Laws 123 Gualtiero Badin Fulvio Crisciani Universität Hamburg University of Trieste Hamburg Trieste Germany Italy ISSN 1866-8348 ISSN 1866-8356 (electronic) Advances in Geophysical and Environmental Mechanics and Mathematics ISBN 978-3-319-59694-5 ISBN 978-3-319-59695-2 (eBook) DOI 10.1007/978-3-319-59695-2 Library of Congress Control Number: 2017949166 © Springer International Publishing AG 2018 This work is subject to copyright. All rights are reserved by the Publisher, whether the whole or part of the material is concerned, specifically the rights of translation, reprinting, reuse of illustrations, recitation, broadcasting, reproduction on microfilms or in any other physical way, and transmission or information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed. The use of general descriptive names, registered names, trademarks, service marks, etc. in this publication does not imply, even in the absence of a specific statement, that such names are exempt from the relevant protective laws and regulations and therefore free for general use. The publisher, the authors and the editors are safe to assume that the advice and information in this book are believed to be true and accurate at the date of publication. -
Calculus of Variations in the Convex Case : an Introduction to Fathi's
Calculus of variations in the convex case : an introduction to Fathi’s weak KAM theorem and Mather’s theory of minimal invariant measures Alain Chenciner, Barcelona july 2004 1st lecture. Calculus of variations in the convex case (local struc- tures). From Euler-Lagrange equations to the Poincar´e-Cartan integral invariant, the Legendre transform and Hamilton’s equations. Exercices. Flows, differential forms, symplectic structures 2nd lecture. The Hamilton-Jacobi equation. The solutions of Hamilton’s equations as characteristics. Lagrangian sub- manifolds and geometric solutions of the Hamilton-Jacobi equation. Caus- tics as an obstruction to the existence of global solutions to the Cauchy problem. Exercices. The geodesic flow on a torus of revolution as an example of a completely integrable system 3rd lecture. Minimizers. Weierstrass theory of minimizers. Minimizing KAM tori, Existence of min- imizers (Tonelli’s theorem) and the Lax-Oleinik semi-group. Exercices. Examples around the pendulum 4th lecture. Global solutions of the Hamilton-Jacobi equation Weak KAM solutions as fixed points of the Lax-Oleinik semi-group; con- vergence of the semi-group in the autonomous case. Conjugate weak KAM solutions. Exercices. Burger’s equation and viscosity solutions. 5th lecture. Mather’s theory. Class A geodesics and minimizing mea- sures. The α and β functions as a kind of integrable skeleton Exercices. The time-periodic case as a generalization of Aubry-Mather the- ory, Birkhoff billiards, Hedlund’s example in higher dimension. 1 1st lecture. Calculus of variations in the convex case (local struc- tures). General convexity hypotheses. M = TI n = IRn/ZZ n is the n-dimen- sional torus (the theory works with an arbitrary compact manifold but the torus will allow us to work with global coordinates). -
Lagrangian and Eulerian Representations of Fluid Flow: Part I, Kinematics and the Equations of Motion
Lagrangian and Eulerian Representations of Fluid Flow: Part I, Kinematics and the Equations of Motion James F. Price MS 29, Clark Laboratory Woods Hole Oceanographic Institution Woods Hole, MA, 02543 http://www.whoi.edu/science/PO/people/jprice [email protected] Version 7.4 September 13, 2005 Summary: This essay introduces the two methods that are commonly used to describe fluid flow, by observing the trajectories of parcels that are carried along with the flow or by observing the fluid velocity at fixed positions. These yield what are commonly termed Lagrangian and Eulerian descriptions. Lagrangian methods are often the most efficient way to sample a fluid domain and the physical conservation laws are inherently Lagrangian since they apply to specific material parcels rather than points in space. It happens, though, that the Lagrangian equations of motion applied to a continuum are quite difficult, and thus almost all of the theory (forward calculation) in fluid dynamics is developed within the Eulerian system. Eulerian solutions may be used to calculate Lagrangian properties, e.g., parcel trajectories, which is often a valuable step in the description of an Eulerian solution. Transformation to and from Lagrangian and Eulerian systems — the central theme of this essay — is thus the foundation of most theory in fluid dynamics and is a routine part of many investigations. The transformation of the Lagrangian conservation laws into the Eulerian equations of motion requires three key results. (1) The first is dubbed the Fundamental Principle of Kinematics; the velocity at a given position and time (the Eulerian velocity) is identically the velocity of the parcel (the Lagrangian velocity) that occupies that position at that time. -
NONLINEAR DISPERSIVE WAVE PROBLEMS Thesis by Jon
NONLINEAR DISPERSIVE WAVE PROBLEMS Thesis by Jon Christian Luke In Partial Fulfillment of the Requirements For the Degree of Doctor of Philosophy California Institute of Technology Pasadena, California 1966 (Submitted April 4, 1966) -ii ACKNOWLEDGMENTS The author expresses his thanks to Professor G. B. Whitham, who suggested the problems treated in this dissertation, and has made available various preliminary calculations, preprints of papers, and lectur~ notes. In addition, Professor Whitham has given freely of his time for useful and enlightening discussions and has offered timely advice, encourageme.nt, and patient super vision. Others who have assisted the author by suggestions or con structive criticism are Mr. G. W. Bluman and Mr. R. Seliger of the California Institute of Technology and Professor J. Moser of New York University. The author gratefully acknowledges the National Science Foundation Graduate Fellowship that made possible his graduate education. J. C. L. -iii ABSTRACT The nonlinear partial differential equations for dispersive waves have special solutions representing uniform wavetrains. An expansion procedure is developed for slowly varying wavetrains, in which full nonl~nearity is retained but in which the scale of the nonuniformity introduces a small parameter. The first order results agree with the results that Whitham obtained by averaging methods. The perturbation method provides a detailed description and deeper understanding, as well as a consistent development to higher approximations. This method for treating partial differ ential equations is analogous to the "multiple time scale" meth ods for ordinary differential equations in nonlinear vibration theory. It may also be regarded as a generalization of geomet r i cal optics to nonlinear problems. -
Interactions and Resonances
A Macroscopic Plasma Lagrangian and its Application to Wave Interactions and Resonances by Yueng-Kay Martin Peng June 1974 SUIPR Report No. 575 National Aeronautics and Space Administration Grant NGL 05-020-176 National Science Foundation Grant GK-32788X (NASA-CR-138649) A MACROSCOPIC PLASMA N74-27231 LAGRANGIAN AND ITS APPLICATION TO WAVE INTERACTIOUS AND RESONANCES (Stanford Univ.) 262 p HC $16.25 CSCL 201 Unclas G3/25 41289 INSTITUTE FOR PLASMA RESEARCH STANFORD UNIVERSITY, STANFORD, CALIFORNIA NIZ~a A MACROSCOPIC PLASMA LAGRANGIAN AND ITS APPLICATION TO WAVE INTERACTIONS AND RESONANCES by Yueng-Kay Martin Peng National Aeronautics and Space Administration Grant NGL 05-020-176 National Science Foundation Grant GK-32788X SUIPR Report No. 575 June 1974 Institute for Plasma Research Stanford University Stanford, California I A MACROSCOPIC PLASMA LAGRANGIAN AND ITS APPLICATION TO WAVE INTERACTIONS AND RESONANCES by Yueng-Kay Martin Peng Institute for Plasma Research Stanford University Stanford, California 94305 ABSTRACT This thesis is concerned with derivation of a macroscopic plasma Lagrangian, and its application to the description of nonlinear three- wave interaction in a homogeneous plasma and linear resonance oscilla- tions in a inhomogeneous plasma. One approach to obtain -the--Lagrangian is via the inverse problem of the calculus of variations for arbitrary first and second order quasilinear partial differential systems. Necessary and sufficient conditions for the given equations to be Euler-Lagrange equations of a Lagrangian are obtained. These conditions are then used to determine the transformations that convert some classes of non-Euler-Lagrange equations to Euler-Lagrange equation form. The Lagrangians for a linear resistive transmission line and a linear warm collisional plasma are derived as examples. -
Lectures in Elementary Fluid Dynamics: Physics, Mathematics and Applications James M
University of Kentucky UKnowledge Mechanical Engineering Textbook Gallery Mechanical Engineering 2009 Lectures In Elementary Fluid Dynamics: Physics, Mathematics and Applications James M. McDonough University of Kentucky, [email protected] Right click to open a feedback form in a new tab to let us know how this document benefits oy u. Follow this and additional works at: https://uknowledge.uky.edu/me_textbooks Part of the Mechanical Engineering Commons Recommended Citation McDonough, James M., "Lectures In Elementary Fluid Dynamics: Physics, Mathematics and Applications" (2009). Mechanical Engineering Textbook Gallery. 1. https://uknowledge.uky.edu/me_textbooks/1 This Book is brought to you for free and open access by the Mechanical Engineering at UKnowledge. It has been accepted for inclusion in Mechanical Engineering Textbook Gallery by an authorized administrator of UKnowledge. For more information, please contact [email protected]. LECTURES IN ELEMENTARY FLUID DYNAMICS: Physics, Mathematics and Applications J. M. McDonough Departments of Mechanical Engineering and Mathematics University of Kentucky, Lexington, KY 40506-0503 c 1987, 1990, 2002, 2004, 2009 Contents 1 Introduction 1 1.1 ImportanceofFluids.............................. ...... 1 1.1.1 Fluidsinthepuresciences. ...... 2 1.1.2 Fluidsintechnology .. .. .. .. .. .. .. .. .... 3 1.2 TheStudyofFluids ................................ .... 4 1.2.1 Thetheoreticalapproach . ..... 5 1.2.2 Experimentalfluiddynamics . ..... 6 1.2.3 Computationalfluiddynamics . ..... 6 1.3 OverviewofCourse............................... -
An Essay on Lagrangian and Eulerian Kinematics of Fluid Flow
Lagrangian and Eulerian Representations of Fluid Flow: Kinematics and the Equations of Motion James F. Price Woods Hole Oceanographic Institution, Woods Hole, MA, 02543 [email protected], http://www.whoi.edu/science/PO/people/jprice June 7, 2006 Summary: This essay introduces the two methods that are widely used to observe and analyze fluid flows, either by observing the trajectories of specific fluid parcels, which yields what is commonly termed a Lagrangian representation, or by observing the fluid velocity at fixed positions, which yields an Eulerian representation. Lagrangian methods are often the most efficient way to sample a fluid flow and the physical conservation laws are inherently Lagrangian since they apply to moving fluid volumes rather than to the fluid that happens to be present at some fixed point in space. Nevertheless, the Lagrangian equations of motion applied to a three-dimensional continuum are quite difficult in most applications, and thus almost all of the theory (forward calculation) in fluid mechanics is developed within the Eulerian system. Lagrangian and Eulerian concepts and methods are thus used side-by-side in many investigations, and the premise of this essay is that an understanding of both systems and the relationships between them can help form the framework for a study of fluid mechanics. 1 The transformation of the conservation laws from a Lagrangian to an Eulerian system can be envisaged in three steps. (1) The first is dubbed the Fundamental Principle of Kinematics; the fluid velocity at a given time and fixed position (the Eulerian velocity) is equal to the velocity of the fluid parcel (the Lagrangian velocity) that is present at that position at that instant. -
Dynamics of Ideal Fluids
2 Dynamics of Ideal Fluids The basic goal of any fluid-dynamical study is to provide (1) a complete description of the motion of the fluid at any instant of time, and hence of the kinematics of the flow, and (2) a description of how the motion changes in time in response to applied forces, and hence of the dynamics of the flow. We begin our study of astrophysical fluid dynamics by analyzing the motion of a compressible ideal fluid (i.e., a nonviscous and nonconducting gas); this allows us to formulate very simply both the basic conservation laws for the mass, momentum, and energy of a fluid parcel (which govern its dynamics) and the essentially geometrical relationships that specify its kinematics. Because we are concerned here with the macroscopic proper- ties of the flow of a physically uncomplicated medium, it is both natural and advantageous to adopt a purely continuum point of view. In the next chapter, where we seek to understand the important role played by internal processes of the gas in transporting energy and momentum within the fluid, we must carry out a deeper analysis based on a kinetic-theory view; even then we shall see that the continuum approach yields useful results and insights. We pursue this line of inquiry even further in Chapters 6 and 7, where we extend the analysis to include the interaction between radiation and both the internal state, and the macroscopic dynamics, of the material. 2.1 Kinematics 15. Veloci~y and Acceleration 1n developing descriptions of fluid motion it is fruitful to work in two different frames of reference, each of which has distinct advantages in certain situations. -
Lagrangian and Eulerian Representations of Fluid Flow: James F
Lagrangian and Eulerian Representations of Fluid Flow: James F. Price MS 29, Clark Laboratory Woods Hole Oceanographic Institution Woods Hole, Massachusetts, USA, 02543 http://www.whoi.edu/science/PO/people/jprice [email protected] Version 3.5 December 22, 2004 Summary: This essay considers the two major ways that the motion of a fluid continuum may be described, either by observing or predicting the trajectories of parcels that are carried about with the flow – which yields a Lagrangian or material representation of the flow — or by observing or predicting the fluid velocity at fixed points in space — which yields an Eulerian or field representation of the flow. Lagrangian methods are often the most efficient way to sample a fluid domain and most of the physical conservation laws begin with a Lagrangian perspective. Nevertheless, almost all of the theory in fluid dynamics is developed in Eulerian or field form. The premise of this essay is that it is helpful to understand both systems, and the transformation between systems is the central theme. The transformation from a Lagrangian to an Eulerian system requires three key results. 1) The first is dubbed the Fundamental Principle of Kinematics; the velocity at a given position and time (sometimes called the Eulerian velocity) is equal to the velocity of the parcel that occupies that position at that time (often called the Lagrangian velocity). 2) The material or substantial derivative relates the time rate of change observed following a moving parcel to the time rate of change observed at a fixed position; D()/Dt = ∂()/∂t + V ·∇(), where the advective rate of change is in field coordinates. -
Particle Motion Near the Resonant Surface of a High-Frequency Wave in a Magnetized Plasma
INVESTIGACION´ REVISTA MEXICANA DE FISICA´ 48 (3) 239–249 JUNIO 2002 Particle motion near the resonant surface of a high-frequency wave in a magnetized plasma J. J. Martinell Instituto de Ciencias Nucleares, Universidad Nacional Autonoma´ de Mexico´ A. Postal 70-543, 04510 Mexico´ D.F. e-mail: [email protected] Recibido el 11 de enero de 2002; aceptado el 4 de febrero de 2002 The motion of single charged particles in a magnetized plasma is studied using a Lagrangian formalism, applied to the average over a gyro- period, in the presence of an electromagnetic wave that is being resonantly absorbed by the medium. Near the resonance surface the wave amplitude has a gradient and the resulting particle drifts are shown to be consistent with the existence of a ponderomotive force, produced by the wave-field-gradient. The orbits are also obtained numerically to show how the drifting motion arises, and to study the case of high field-gradients, which is not described with the formal analysis. Keywords: Charged particle orbits; electromagnetic waves in plasmas; lagrangian mechanics. Se estudia el movimiento de part´ıculas cargadas individuales en un plasma magnetizado con un formalismo Lagrangiano, aplicado al prome- dio sobre un per´ıodo de giro, en presencia de una onda electromagnetica´ que es absorbida de manera resonante por el medio. Cerca de la superficie de resonancia la amplitud de la onda tiene un gradiente y se muestra que los movimientos de deriva resultantes son consistentes con la existencia de una fuerza ponderomotriz, producida por el gradiente del campo de la onda. -
Fluid Kinematics 4
cen72367_ch04.qxd 10/29/04 2:23 PM Page 121 CHAPTER FLUID KINEMATICS 4 luid kinematics deals with describing the motion of fluids without nec- essarily considering the forces and moments that cause the motion. In OBJECTIVES Fthis chapter, we introduce several kinematic concepts related to flow- When you finish reading this chapter, you ing fluids. We discuss the material derivative and its role in transforming should be able to the conservation equations from the Lagrangian description of fluid flow I Understand the role of the (following a fluid particle) to the Eulerian description of fluid flow (pertain- material derivative in ing to a flow field). We then discuss various ways to visualize flow fields— transforming between Lagrangian and Eulerian streamlines, streaklines, pathlines, timelines, and optical methods schlieren descriptions and shadowgraph—and we describe three ways to plot flow data—profile I Distinguish between various plots, vector plots, and contour plots. We explain the four fundamental kine- types of flow visualizations matic properties of fluid motion and deformation—rate of translation, rate and methods of plotting the of rotation, linear strain rate, and shear strain rate. The concepts of vortic- characteristics of a fluid flow ity, rotationality, and irrotationality in fluid flows are also discussed. I Have an appreciation for the Finally, we discuss the Reynolds transport theorem (RTT), emphasizing its many ways that fluids move role in transforming the equations of motion from those following a system and deform to those pertaining to fluid flow into and out of a control volume. The anal- I Distinguish between rotational ogy between material derivative for infinitesimal fluid elements and RTT for and irrotational regions of flow based on the flow property finite control volumes is explained. -
Lectures on Dynamical Meteorology
LECTURES ON DYNAMICAL METEOROLOGY Roger K. Smith Version: June 16, 2014 Contents 1 INTRODUCTION 5 1.1 Scales ................................... 6 2 EQUILIBRIUM AND STABILITY 9 3 THE EQUATIONS OF MOTION 16 3.1 Effectivegravity.............................. 16 3.2 TheCoriolisforce............................. 16 3.3 Euler’s equation in a rotating coordinate system . 18 3.4 Centripetalacceleration .. .. .. 19 3.5 Themomentumequation.. .. .. 20 3.6 TheCoriolisforce............................. 20 3.7 Perturbationpressure. .. .. .. 21 3.8 Scale analysis of the equation of motion . 22 3.9 Coordinate systems and the earth’s sphericity . 23 3.10 Scale analysis of the equations for middle latitude synoptic systems . 25 4 GEOSTROPHIC FLOWS 28 4.1 TheTaylor-ProudmanTheorem . 30 4.2 Blocking.................................. 34 4.3 Analogy between blocking and axial Taylor columns . 35 4.4 Stability of a rotating fluid . 38 4.5 Vortexflows: thegradientwindequation . 38 4.6 Theeffectsofstratification. 41 4.7 Thermaladvection ............................ 45 4.8 Thethermodynamicequation . 46 4.9 Pressurecoordinates ........................... 47 4.10 Thicknessadvection. .. .. .. 48 4.11 Generalizedthermalwindequation . 49 5 FRONTS, EKMAN BOUNDARY LAYERS AND VORTEX FLOWS 54 5.1 Fronts ................................... 54 5.2 Margules’model.............................. 54 5.3 Viscous boundary layers: Ekman’s solution . 59 2 CONTENTS 3 5.4 Vortexboundarylayers. .. .. .. 63 6 THE VORTICITY EQUATION FOR A HOMOGENEOUS FLUID 67 6.1 Planetary,orRossbyWaves . 68 6.2 Largescaleflowoveramountainbarrier . 74 6.3 Winddrivenoceancurrents . 75 6.4 Topographicwaves ............................ 79 6.5 Continentalshelfwaves. .. .. .. 81 7 THE VORTICITY EQUATION IN A ROTATING STRATIFIED FLUID 83 7.1 The vorticity equation for synoptic-scale atmospheric motions . ... 85 8 QUASI-GEOSTROPHIC MOTION 89 8.1 More on the approximated thermodynamic equation . 92 8.2 The quasi-geostrophic equation for a compressible atmosphere ...