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an introduction to dynamic meteorology

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  • Contents

  • Preface

  • 1. Introduction

    • 1.1 THE ATMOSPHERIC CONTINUUM

    • 1.2 PHYSICAL DIMENSIONS AND UNITS

    • 1.3 SCALE ANALYSIS

    • 1.4 FUNDAMENTAL FORCES

      • 1.4.1 Pressure Gradient Force

      • 1.4.2 Gravitational Force

      • 1.4.3 Viscous Force

    • 1.5 NONINERTIAL REFERENCE FRAMES AND “APPARENT” FORCES

      • 1.5.1 Centripetal Acceleration and Centrifugal Force

      • 1.5.2 Gravity Force

      • 1.5.3 The Coriolis Force and the Curvature Effect

      • 1.5.4 Constant Angular Momentum Oscillations

    • 1.6 STRUCTURE OF THE STATIC ATMOSPHERE

      • 1.6.1 The Hydrostatic Equation

      • 1.6.2 Pressure as a Vertical Coordinate

      • 1.6.3 A Generalized Vertical Coordinate

    • PROBLEMS

    • MATLAB EXERCISES

    • Suggested References

  • 2. Basic Conservation Laws

    • 2.1 TOTAL DIFFERENTIATION

      • 2.1.1 Total Differentiation of a Vector in a Rotating System

    • 2.2 THE VECTORIAL FORM OF THE MOMENTUM EQUATION IN ROTATING COORDINATES

    • 2.3 COMPONENT EQUATIONS IN SPHERICAL COORDINATES

    • 2.4 SCALE ANALYSIS OF THE EQUATIONS OF MOTION

      • 2.4.1 Geostrophic Approximation and GeostrophicWind

      • 2.4.2 Approximate Prognostic Equations; the Rossby Number

      • 2.4.3 The Hydrostatic Approximation

    • 2.5 THE CONTINUITY EQUATION

      • 2.5.1 An Eulerian Derivation

      • 2.5.2 A Lagrangian Derivation

      • 2.5.3 Scale Analysis of the Continuity Equation

    • 2.6 THE THERMODYNAMIC ENERGY EQUATION

    • 2.7 THERMODYNAMICS OF THE DRY ATMOSPHERE

      • 2.7.1 Potential Temperature

      • 2.7.2 The Adiabatic Lapse Rate

      • 2.7.3 Static Stability

      • 2.7.4 Scale Analysis of the Thermodynamic Energy Equation

    • PROBLEMS

    • MATLAB EXERCISES

    • Suggested References

  • 3. Elementary Applications of the Basic Equations

    • 3.1 BASIC EQUATIONS IN ISOBARIC COORDINATES

      • 3.1.1 The Horizontal Momentum Equation

      • 3.1.2 The Continuity Equation

      • 3.1.3 The Thermodynamic Energy Equation

    • 3.2 BALANCED FLOW

      • 3.2.1 Natural Coordinates

      • 3.2.2 Geostrophic Flow

      • 3.2.3 Inertial Flow

      • 3.2.4 Cyclostrophic Flow

      • 3.2.5 The GradientWind Approximation

    • 3.3 TRAJECTORIES AND STREAMLINES

    • 3.4 THE THERMAL WIND

      • 3.4.1 Barotropic and Baroclinic Atmospheres

    • 3.5 VERTICAL MOTION

      • 3.5.1 The Kinematic Method

      • 3.5.2 The Adiabatic Method

    • 3.6 SURFACE PRESSURE TENDENCY

    • PROBLEMS

    • MATLAB EXERCISES

  • 4. Circulation and Vorticity

    • 4.1 THE CIRCULATION THEOREM

    • 4.2 VORTICITY

      • 4.2.1 Vorticity in Natural Coordinates

    • 4.3 POTENTIAL VORTICITY

    • 4.4 THE VORTICITY EQUATION

      • 4.4.1 Cartesian Coordinate Form

      • 4.4.2 The Vorticity Equation in Isobaric Coordinates

      • 4.4.3 Scale Analysis of the Vorticity Equation

    • 4.5 VORTICITY IN BAROTROPIC FLUIDS

      • 4.5.1 The Barotropic (Rossby) Potential Vorticity Equation

      • 4.5.2 The Barotropic Vorticity Equation

    • 4.6 THEBAROCLINIC (ERTEL) POTENTIALVORTICITYEQUATION

      • 4.6.1 Equations of Motion in Isentropic Coordinates

      • 4.6.2 The Potential Vorticity Equation

      • 4.6.3 Integral Constraints on Isentropic Vorticity

    • PROBLEMS

    • MATLAB EXERCISES

    • Suggested References

  • 5. The Planetary Boundary Layer

    • 5.1 ATMOSPHERIC TURBULENCE

      • 5.1.1 The Boussinesq Approximation

      • 5.1.2 Reynolds Averaging

    • 5.2 TURBULENT KINETIC ENERGY

    • 5.3 PLANETARY BOUNDARY LAYER MOMENTUM EQUATIONS

      • 5.3.1 Well-Mixed Boundary Layer

      • 5.3.2 The Flux–Gradient Theory

      • 5.3.3 The Mixing Length Hypothesis

      • 5.3.4 The Ekman Layer

      • 5.3.5 The Surface Layer

      • 5.3.6 The Modified Ekman Layer

    • 5.4 SECONDARY CIRCULATIONS AND SPIN DOWN

    • PROBLEMS

    • MATLAB EXERCISES

    • Suggested References

  • 6. Synoptic-Scale Motions I: Quasi- Geostrophic Analysis

    • 6.1 THE OBSERVED STRUCTURE OF EXTRATROPICAL CIRCULATIONS

    • 6.2 THE QUASI-GEOSTROPHIC APPROXIMATION

      • 6.2.1 Scale Analysis in Isobaric Coordinates

      • 6.2.2 The Quasi-Geostrophic Vorticity Equation

    • 6.3 QUASI-GEOSTROPHIC PREDICTION

      • 6.3.1 Geopotential Tendency

      • 6.3.2 The Quasi-Geostrophic Potential Vorticity Equation

      • 6.3.3 Potential Vorticity Inversion

      • 6.3.4 Vertical Coupling Through Potential Vorticity

    • 6.4 DIAGNOSIS OF THE VERTICAL MOTION

      • 6.4.1 The Traditional Omega Equation

      • 6.4.2 The Q Vector

      • 6.4.3 The Ageostrophic Circulation

    • 6.5 IDEALIZED MODEL OF A BAROCLINIC DISTURBANCE

    • PROBLEMS

    • MATLAB EXERCISES

    • Suggested References 6

  • 7. Atmospheric Oscillations: Linear Perturbation Theory

    • 7.1 THE PERTURBATION METHOD

    • 7.2 PROPERTIES OFWAVES

      • 7.2.1 Fourier Series

      • 7.2.2 Dispersion and Group Velocity

    • 7.3 SIMPLEWAVE TYPES

      • 7.3.1 Acoustic or SoundWaves

      • 7.3.2 ShallowWater GravityWaves

    • 7.4 INTERNAL GRAVITY (BUOYANCY) WAVES

      • 7.4.1 Pure Internal GravityWaves

      • 7.4.2 TopographicWaves

    • 7.5 GRAVITYWAVES MODIFIED BY ROTATION

      • 7.5.1 Pure Inertial Oscillations

      • 7.5.2 Inertia–GravityWaves

    • 7.6 ADJUSTMENT TO GEOSTROPHIC BALANCE

    • 7.7 ROSSBYWAVES

      • 7.7.1 Free Barotropic RossbyWaves

      • 7.7.2 Forced Topographic RossbyWaves

    • PROBLEMS

    • MATLAB EXERCISES

    • Suggested References

  • 8. Synoptic-Scale Motions II: Baroclinic Instability

    • 8.1 HYDRODYNAMIC INSTABILITY

    • 8.2 NORMAL MODE BAROCLINIC INSTABILITY: A TWO-LAYER MODEL

      • 8.2.1 Linear Perturbation Analysis

      • 8.2.2 Vertical Motion in BaroclinicWaves

    • 8.3 THE ENERGETICS OF BAROCLINICWAVES

      • 8.3.1 Available Potential Energy

      • 8.3.2 Energy Equations for the Two-Layer Model

    • 8.4 BAROCLINIC INSTABILITY OFA CONTINUOUSLY STRATIFIED ATMOSPHERE

      • 8.4.1 Log-Pressure Coordinates

      • 8.4.2 Baroclinic Instability: The Rayleigh Theorem

      • 8.4.3 The Eady Stability Problem

    • 8.5 GROWTHAND PROPAGATION OF NEUTRAL MODES

      • 8.5.1 Transient Growth of NeutralWaves

      • 8.5.2 Downstream Development

    • PROBLEMS

    • MATLAB EXERCISES

    • Suggested References

  • 9. Mesoscale Circulations

    • 9.1 ENERGY SOURCES FOR MESOSCALE CIRCULATIONS

    • 9.2 FRONTS AND FRONTOGENESIS

      • 9.2.1 The Kinematics of Frontogenesis

      • 9.2.2 Semigeostrophic Theory

      • 9.2.3 Cross-Frontal Circulation

    • 9.3 SYMMETRIC BAROCLINIC INSTABILITY

    • 9.4 MOUNTAINWAVES

      • 9.4.1 Flow over Isolated Ridges

      • 9.4.2 LeeWaves

      • 9.4.3 DownslopeWindstorms

    • 9.5 CUMULUS CONVECTION

      • 9.5.1 Equivalent Potential Temperature

      • 9.5.2 The Pseudoadiabatic Lapse Rate

      • 9.5.3 Conditional Instability

      • 9.5.4 Convective Available Potential Energy (CAPE)

      • 9.5.5 Entrainment

    • 9.6 CONVECTIVE STORMS

      • 9.6.1 Development of Rotation in Supercell Thunderstorms

      • 9.6.2 The Right-Moving Storm

    • 9.7 HURRICANES

      • 9.7.1 Dynamics of Mature Hurricanes

      • 9.7.2 Hurricane Development

    • PROBLEMS

    • MATLAB EXERCISES

    • Suggested References

  • 10. The General Circulation

    • 10.1 THE NATURE OF THE PROBLEM

    • 10.2 THE ZONALLY AVERAGED CIRCULATION

      • 10.2.1 The Conventional Eulerian Mean

      • 10.2.2 The Transformed Eulerian Mean (TEM)

      • 10.2.3 The Zonal-Mean Potential Vorticity Equation

    • 10.3 THE ANGULAR MOMENTUM BUDGET

      • 10.3.1 Sigma Coordinates

      • 10.3.2 The Zonal-Mean Angular Momentum

    • 10.4 THE LORENZ ENERGY CYCLE

    • 10.5 LONGITUDINALLY DEPENDENT TIME-AVERAGED FLOW

      • 10.5.1 Stationary RossbyWaves

      • 10.5.2 Jetstream and Storm Tracks

    • 10.6 LOW-FREQUENCY VARIABILITY

      • 10.6.1 Climate Regimes

      • 10.6.2 Annular Modes

      • 10.6.3 Sea Surface Temperature Anomalies

    • 10.7 LABORATORYSIMULATIONOFTHEGENERALCIRCULATION

    • 10.8 NUMERICAL SIMULATION OF THE GENERAL CIRCULATION

      • 10.8.1 The Development of AGCMs

      • 10.8.2 Dynamical Formulation

      • 10.8.3 Physical Processes and Parameterizations

      • 10.8.4 The NCAR Climate System Model

    • PROBLEMS

    • MATLAB EXERCISES

    • Suggested References

  • 11. Tropical Dynamics

    • 11.1 THE OBSERVED STRUCTURE OF LARGE-SCALE TROPICAL CIRCULATIONS

      • 11.1.1 The Intertropical Convergence Zone

      • 11.1.2 EquatorialWave Disturbances

      • 11.1.3 AfricanWave Disturbances

      • 11.1.4 Tropical Monsoons

      • 11.1.5 TheWalker Circulation

      • 11.1.6 El Ni ˜ no and the Southern Oscillation

      • 11.1.7 Equatorial Intraseasonal Oscillation

    • 11.2 SCALE ANALYSIS OF LARGE-SCALE TROPICAL MOTIONS

    • 11.3 CONDENSATION HEATING

    • 11.4 EQUATORIALWAVE THEORY

      • 11.4.1 Equatorial Rossby and Rossby–Gravity Modes

      • 11.4.2 Equatorial KelvinWaves

    • 11.5 STEADY FORCED EQUATORIAL MOTIONS

    • PROBLEMS

    • MATLAB EXERCISES

    • Suggested References

  • 12. Middle Atmosphere Dynamics

    • 12.1 STRUCTURE AND CIRCULATION OF THE MIDDLE ATMOSPHERE

    • 12.2 THE ZONAL-MEAN CIRCULATION OF THE MIDDLE ATMOSPHERE

      • 12.2.1 Lagrangian Motion of Air Parcels

      • 12.2.2 The Transformed Eulerian Mean

      • 12.2.3 Zonal-Mean Transport

    • 12.3 VERTICALLY PROPAGATING PLANETARYWAVES

      • 12.3.1 Linear RossbyWaves

      • 12.3.2 RossbyWavebreaking

    • 12.4 SUDDEN STRATOSPHERICWARMINGS

    • 12.5 WAVES IN THE EQUATORIAL STRATOSPHERE

      • 12.5.1 Vertically Propagating KelvinWaves

      • 12.5.2 Vertically Propagating Rossby–GravityWaves

      • 12.5.3 Observed EquatorialWaves

    • 12.6 THE QUASI-BIENNIAL OSCILLATION

    • 12.7 TRACE CONSTITUENT TRANSPORT

      • 12.7.1 Dynamical Tracers

      • 12.7.2 Chemical Tracers

      • 12.7.3 Transport in the Stratosphere

    • PROBLEMS

    • MATLAB EXERCISES

    • Suggested References 12

  • 13. Numerical Modeling and Prediction

    • 13.1 HISTORICAL BACKGROUND

    • 13.2 FILTERING METEOROLOGICAL NOISE

    • 13.3 NUMERICAL APPROXIMATION OF THE EQUATIONS OF MOTION

      • 13.3.1 Finite Differences

      • 13.3.2 Centered Differences: Explicit Time Differencing

      • 13.3.3 Computational Stability

      • 13.3.4 Implicit Time Differencing

      • 13.3.5 The Semi-Lagrangian Integration Method

      • 13.3.6 Truncation Error

    • 13.4 THE BAROTROPIC VORTICITY EQUATION IN FINITE DIFFERENCES

    • 13.5 THE SPECTRAL METHOD

      • 13.5.1 The Barotropic Vorticity Equation in Spherical Coordinates

      • 13.5.2 Rossby–HaurwitzWaves

      • 13.5.3 The Spectral Transform Method

    • 13.6 PRIMITIVE EQUATION MODELS

      • 13.6.1 The Ecmwf Grid Point Model

      • 13.6.2 Spectral Models

      • 13.6.3 Physical Parameterizations

    • 13.7 DATA ASSIMILATION

      • 13.7.1 The Initialization Problem

      • 13.7.2 Nonlinear Normal Mode Initialization

      • 13.7.3 Four-Dimensional Data Assimilation

    • 13.8 PREDICTABILITY AND ENSEMBLE PREDICTION SYSTEMS

    • PROBLEMS

    • MATLAB EXERCISES

    • Suggested References

  • Appendix A: Useful Constants and Parameters

  • Appendix B: List of Symbols

  • Appendix C: Vector Analysis

    • C.1 VECTOR IDENTITIES

    • C.2 INTEGRAL THEOREMS

    • C.3 VECTOR OPERATIONS IN VARIOUS COORDINATE SYSTEMS

  • Appendix D: Moisture Variables

    • D.1 EQUIVALENT POTENTIAL TEMPERATURE

    • D.2 PSEUDOADIABATIC LAPSE RATE

  • Appendix E: Standard Atmosphere Data

  • Appendix F: Symmetric Baroclinic Oscillations

  • Bibliography

  • Index

Nội dung

[...]... vector g* and gravity g For an idealized homogeneous spherical earth, g* would be directed toward the center of the earth In reality, g* does not point exactly to the center except at the equator and the poles Gravity, g, is the vector sum of g* and the centrifugal force and is perpendicular to the level surface of the earth, which approximates an oblate spheroid surfaces slope upward toward the equator... a distance r (1.3) January 27, 2004 13:54 Elsevier/AID 8 aid 1 introduction In dynamic meteorology it is customary to use the height above mean sea level as a vertical coordinate If the mean radius of the earth is designated by a and the distance above mean sea level is designated by z, then neglecting the small departure of the shape of the earth from sphericity, r = a + z Therefore, (1.3) can be... techniques and ensemble forecasting Acknowledgments: I am indebted to a large number of colleagues and students for their continuing interest, suggestions, and help with various figures I am particularly grateful to Drs Dale Durran, Greg Hakim, Todd Mitchell, Adrian Simmons, David Thompson, and John Wallace for various suggestions and figures January 27, 2004 13:54 Elsevier/AID aid C H A P T E R 1 Introduction. .. force proportional to their masses and inversely proportional to the square of the distance separating them Thus, if two mass elements M and m are separated by a distance r ≡ |r| (with the vector r directed toward m as shown in Fig 1.2), then the force exerted by mass M on mass m due to gravitation is GMm r Fg = − 2 (1.2) r r where G is a universal constant called the gravitational constant The law of... still fundamental to the understanding of large-scale extratropical motions This chapter has been revised to provide increased emphasis on the role of potential vorticity and potential vorticity inversion The presentation of the omega equation and the Q vector has been revised and improved In Chapter 9, the discussions of fronts, symmetric instability, and hurricanes have all been expanded and improved... of view of an observer in inertial space the speed of the ball is constant, but its direction of travel is continuously changing so that its velocity is not constant To compute the acceleration we consider the change in velocity δV that occurs for a time increment δt during which the ball rotates through an angle δθ as shown in Fig 1.5 Because δθ is also the angle between the vectors V and V + δV,... Therefore, in order to apply Newton’s second law to describe the motion relative to this rotating coordinate system, we must include an additional apparent force, the centrifugal force, which just balances the force of the string on the ball Thus, the centrifugal force is equivalent to the inertial reaction of the ball on the string and just equal and opposite to the centripetal acceleration To summarize,... of important derived units have special names and symbols Those that are commonly used in dynamic meteorology are indicated in Table 1.2 In addition, the supplementary unit designating a plane angle, the radian (rad), is required for expressing angular velocity (rad s−1 ) in the SI system.1 In order to keep numerical values within convenient limits, it is conventional to use decimal multiples and submultiples... must change Thus, the object behaves as though a zonally directed deflection force were acting on it The form of the zonal deflection force can be obtained by equating the total angular momentum at the initial distance R to the total angular momentum at the displaced distance R + δR: + u R2 = R + u + δu R + δR (R + δR)2 where δu is the change in eastward relative velocity after displacement Expanding... (h), and day (d) may be used in preference to the second in order to express quantities in convenient numerical values 2 The hectopascal (hPa) is the preferred SI unit for pressure Many meteorologists, however, are still accustomed to using the millibar (mb), which is numerically equivalent to 1 hPa For conformity with current best practice, pressures in this text will generally be expressed in hectopascals . Paris San Diego San Francisco Singapore Sydney Tokyo January 24, 2004 12:0 Elsevier/AID aid Senior Editor, Earth Sciences Frank Cynar Editorial Coordinator Jennifer Helé Senior Marketing Manager. Elsevier/AID aid AN INTRODUCTION TO DYNAMIC METEOROLOGY Fourth Edition JAMES R. HOLTON Department of Atmospheric Sciences University of Washington Seattle,Washington Amsterdam Boston Heidelberg. publication may be reproduced or transmitted in any form or by any means, electronic or mechanical, including photocopy, recording, or any information storage and retrieval system, without permission

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