Optical Metrology Third Edition

Total Page:16

File Type:pdf, Size:1020Kb

Optical Metrology Third Edition Optical Metrology Third Edition Kjell J. Gasvik˚ Spectra Vision AS, Trondheim, Norway Optical Metrology Third Edition Optical Metrology Third Edition Kjell J. Gasvik˚ Spectra Vision AS, Trondheim, Norway Copyright 2002 John Wiley & Sons Ltd, The Atrium, Southern Gate, Chichester, West Sussex PO19 8SQ, England Telephone (+44) 1243 779777 Email (for orders and customer service enquiries): [email protected] Visit our Home Page on www.wileyeurope.com or www.wiley.com All Rights Reserved. No part of this publication may be reproduced, stored in a retrieval system or transmitted in any form or by any means, electronic, mechanical, photocopying, recording, scanning or otherwise, except under the terms of the Copyright, Designs and Patents Act 1988 or under the terms of a licence issued by the Copyright Licensing Agency Ltd, 90 Tottenham Court Road, London W1T 4LP, UK, without the permission in writing of the Publisher. Requests to the Publisher should be addressed to the Permissions Department, John Wiley & Sons Ltd, The Atrium, Southern Gate, Chichester, West Sussex PO19 8SQ, England, or emailed to [email protected], or faxed to (+44) 1243 770571. This publication is designed to provide accurate and authoritative information in regard to the subject matter covered. It is sold on the understanding that the Publisher is not engaged in rendering professional services. If professional advice or other expert assistance is required, the services of a competent professional should be sought. Other Wiley Editorial Offices John Wiley & Sons Inc., 111 River Street, Hoboken, NJ 07030, USA Jossey-Bass, 989 Market Street, San Francisco, CA 94103-1741, USA Wiley-VCH Verlag GmbH, Boschstr. 12, D-69469 Weinheim, Germany John Wiley & Sons Australia Ltd, 33 Park Road, Milton, Queensland 4064, Australia John Wiley & Sons (Asia) Pte Ltd, 2 Clementi Loop #02-01, Jin Xing Distripark, Singapore 129809 John Wiley & Sons Canada Ltd, 22 Worcester Road, Etobicoke, Ontario, Canada M9W 1L1 British Library Cataloguing in Publication Data A catalogue record for this book is available from the British Library ISBN 0-470-84300-4 Typeset in 10/12pt Times by Laserwords Private Limited, Chennai, India Printed and bound in Great Britain by Antony Rowe Ltd, Chippenham, Wiltshire This book is printed on acid-free paper responsibly manufactured from sustainable forestry in which at least two trees are planted for each one used for paper production. Contents Preface to the Third Edition xi 1Basics 1 1.1 Introduction 1 1.2 Wave Motion. The Electromagnetic Spectrum 1 1.3 The Plane Wave. Light Rays 3 1.4 Phase Difference 4 1.5 Complex Notation. Complex Amplitude 5 1.6 Oblique Incidence of A Plane Wave 5 1.7 The Spherical Wave 7 1.8 The Intensity 8 1.9 Geometrical Optics 8 1.10 The Simple Convex (Positive) Lens 10 1.11 A Plane-Wave Set-Up 11 2 Gaussian Optics 15 2.1 Introduction 15 2.2 Refraction at a Spherical Surface 15 2.2.1 Examples 19 2.3 The General Image-Forming System 19 2.4 The Image-Formation Process 21 2.5 Reflection at a Spherical Surface 23 2.6 Aspheric Lenses 25 2.7 Stops and Apertures 26 2.8 Lens Aberrations. Computer Lens Design 28 2.9 Imaging and The Lens Formula 29 2.10 Standard Optical Systems 30 2.10.1 Afocal Systems. The Telescope 30 2.10.2 The Simple Magnifier 32 2.10.3 The Microscope 34 vi CONTENTS 3 Interference 37 3.1 Introduction 37 3.2 General Description 37 3.3 Coherence 38 3.4 Interference between two Plane Waves 41 3.4.1 Laser Doppler Velocimetry (LDV) 45 3.5 Interference between other Waves 46 3.6 Interferometry 49 3.6.1 Wavefront Division 50 3.6.2 Amplitude Division 51 3.6.3 The Dual-Frequency Michelson Interferometer 54 3.6.4 Heterodyne (Homodyne) Detection 55 3.7 Spatial and Temporal Coherence 56 3.8 Optical Coherence Tomography 61 4 Diffraction 67 4.1 Introduction 67 4.2 Diffraction from a Single Slit 67 4.3 Diffraction from a Grating 70 4.3.1 The Grating Equation. Amplitude Transmittance 70 4.3.2 The Spatial Frequency Spectrum 73 4.4 Fourier Optics 75 4.5 Optical Filtering 76 4.5.1 Practical Filtering Set-Ups 78 4.6 Physical Optics Description of Image Formation 81 4.6.1 The Coherent Transfer Function 83 4.6.2 The Incoherent Transfer Function 85 4.6.3 The Depth of Focus 88 4.7 The Phase-Modulated Sinusoidal Grating 89 5 Light Sources and Detectors 99 5.1 Introduction 99 5.2 Radiometry. Photometry 99 5.2.1 Lambertian Surface 102 5.2.2 Blackbody Radiator 103 5.2.3 Examples 105 5.3 Incoherent Light Sources 108 5.4 Coherent Light Sources 109 5.4.1 Stimulated Emission 109 5.4.2 Gas Lasers 112 5.4.3 Liquid Lasers 114 5.4.4 Semiconductor Diode Lasers. Light Emitting Diodes 114 5.4.5 Solid-State Lasers 117 5.4.6 Other Lasers 119 CONTENTS vii 5.4.7 Enhancements of Laser Operation 119 5.4.8 Applications 122 5.4.9 The Coherence Length of a Laser 123 5.5 Hologram Recording Media 125 5.5.1 Silver Halide Emulsions 125 5.5.2 Thermoplastic Film 126 5.5.3 Photopolymer Materials 127 5.6 Photoelectric Detectors 127 5.6.1 Photoconductors 128 5.6.2 Photodiodes 129 5.7 The CCD Camera 131 5.7.1 Operating Principles 131 5.7.2 Responsitivity 134 5.8 Sampling 135 5.8.1 Ideal Sampling 135 5.8.2 Non-Ideal Sampling 138 5.8.3 Aliasing 139 5.9 Signal Transfer 139 6 Holography 147 6.1 Introduction 147 6.2 The Holographic Process 147 6.3 An Alternative Description 150 6.4 Uncollimated Reference and Reconstruction Waves 150 6.5 Diffraction Efficiency. The Phase Hologram 153 6.6 Volume Holograms 154 6.7 Stability Requirements 156 6.8 Holographic Interferometry 157 6.8.1 Double-Exposure Interferometry 157 6.8.2 Real-Time Interferometry 157 6.8.3 Analysis of Interferograms 158 6.8.4 Localization of Interference Fringes 161 6.9 Holographic Vibration Analysis 165 6.10 Holographic Interferometry of Transparent Objects 168 7Moire´ Methods. Triangulation 173 7.1 Introduction 173 7.2 Sinusoidal Gratings 173 7.3 Moire´ Between Two Angularly Displaced Gratings 175 7.4 Measurement of In-Plane Deformation and Strains 175 7.4.1 Methods for Increasing the Sensitivity 177 viii CONTENTS 7.5 Measurement of Out-Of-Plane Deformations. Contouring 179 7.5.1 Shadow Moire´ 179 7.5.2 Projected Fringes 180 7.5.3 Vibration Analysis 186 7.5.4 Moire´ Technique by Means of Digital Image Processing 188 7.6 Reflection Moire´ 189 7.7 Triangulation 190 8 Speckle Methods 193 8.1 Introduction 193 8.2 The Speckle Effect 193 8.3 Speckle Size 195 8.4 Speckle Photography 197 8.4.1 The Fourier Fringe Method 197 8.4.2 The Young Fringe Method 201 8.5 Speckle Correlation 203 8.6 Speckle-Shearing Interferometry 208 8.7 White-Light Speckle Photography 212 9 Photoelasticity and Polarized Light 217 9.1 Introduction 217 9.2 Polarized Light 217 9.3 Polarizing Filters 219 9.3.1 The Linear Polarizer 219 9.3.2 Retarders 221 9.4 Unpolarized Light 223 9.5 Reflection and Refraction at an Interface 223 9.6 The Jones Matrix Formalism of Polarized Light 227 9.7 Photoelasticity 230 9.7.1 Introduction 230 9.7.2 The Plane Polariscope 231 9.7.3 The Circular Polariscope 232 9.7.4 Detection of Isochromatics of Fractional Order. Compensation 234 9.8 Holographic Photoelasticity 237 9.9 Three-Dimensional Photoelasticity 239 9.9.1 Introduction 239 9.9.2 The Frozen Stress Method 241 9.9.3 The Scattered Light Method 242 9.10 Ellipsometry 245 10 Digital Image Processing 249 10.1 Introduction 249 10.2 The Frame Grabber 249 CONTENTS ix 10.3 Digital Image Representation 251 10.4 Camera Calibration 251 10.4.1 Lens Distortion 252 10.4.2 Perspective Transformations 254 10.5 Image Processing 254 10.5.1 Contrast Stretching 255 10.5.2 Neighbourhood Operations. Convolution 256 10.5.3 Noise Suppression 257 10.5.4 Edge Detection 259 10.6 The Discrete Fourier Transform (DFT) and the FFT 262 11 Fringe Analysis 269 11.1 Introduction 269 11.2 Intensity-Based Analysis Methods 269 11.2.1 Introduction 269 11.2.2 Prior Knowledge 270 11.2.3 Fringe Tracking and Thinning 270 11.2.4 Fringe Location by Sub-Pixel Accuracy 273 11.3 Phase-Measurement Interferometry 276 11.3.1 Introduction 276 11.3.2 Principles of TPMI 276 11.3.3 Means of Phase Modulation 279 11.3.4 Different Techniques 279 11.3.5 Errors in TPMI Measurements 281 11.4 Spatial Phase-Measurement Methods 282 11.4.1 Multichannel Interferometer 282 11.4.2 Errors in Multichannel Interferometers 285 11.4.3 Spatial-Carrier Phase-Measurement Method 285 11.4.4 Errors in the Fourier Transform Method 287 11.4.5 Space Domain 289 11.5 Phase Unwrapping 290 11.5.1 Introduction 290 11.5.2 Phase-Unwrapping Techniques 292 11.5.3 Path-Dependent Methods 292 11.5.4 Path-Independent Methods 293 11.5.5 Temporal Phase Unwrapping 295 12 Computerized Optical Processes 297 12.1 Introduction 297 12.2 TV Holography (ESPI) 298 12.3 Digital Holography 301 12.4 Digital Speckle Photography 305 13 Fibre Optics in Metrology 307 13.1 Introduction 307 13.2 Light Propagation through Optical Fibres 307 13.3 Attenuation and Dispersion 310 x CONTENTS 13.4 Different Types of Fibres 313 13.5 Fibre-Optic Sensors 315 13.6 Fibre-Bragg Sensors 318 Appendices A.
Recommended publications
  • Physics-272 Lecture 21
    Physics-272Physics-272 Lecture Lecture 21 21 Description of Wave Motion Electromagnetic Waves Maxwell’s Equations Again ! Maxwell’s Equations James Clerk Maxwell (1831-1879) • Generalized Ampere’s Law • And made equations symmetric: – a changing magnetic field produces an electric field – a changing electric field produces a magnetic field • Showed that Maxwell’s equations predicted electromagnetic waves and c =1/ √ε0µ0 • Unified electricity and magnetism and light . Maxwell’s Equations (integral form) Name Equation Description Gauss’ Law for r r Q Charge and electric Electricity ∫ E ⋅ dA = fields ε0 Gauss’ Law for r r Magnetic fields Magnetism ∫ B ⋅ dA = 0 r r Electrical effects dΦB from changing B Faraday’s Law ∫ E ⋅ ld = − dt field Ampere’s Law r Magnetic effects dΦE from current and (modified by ∫ B ⋅ dl = µ0ic + ε0 Maxwell) dt Changing E field All of electricity and magnetism is summarized by Maxwell’s Equations. On to Waves!! • Note the symmetry now of Maxwell’s Equations in free space, meaning when no charges or currents are present r r r r ∫ E ⋅ dA = 0 ∫ B ⋅ dA = 0 r r dΦ r dΦ ∫ E ⋅ ld = − B B ⋅ dl = µ ε E dt ∫ 0 0 dt • Combining these equations leads to wave equations for E and B, e.g., ∂2E ∂ 2 E x= µ ε x ∂z20 0 ∂ t 2 • Do you remember the wave equation??? 2 2 ∂h1 ∂ h h is the variable that is changing 2= 2 2 in space (x) and time ( t). v is the ∂x v ∂ t velocity of the wave. Review of Waves from Physics 170 2 2 • The one-dimensional wave equation: ∂h1 ∂ h 2= 2 2 has a general solution of the form: ∂x v ∂ t h(x,t) = h1(x − vt ) + h2 (x + vt ) where h1 represents a wave traveling in the +x direction and h2 represents a wave traveling in the -x direction.
    [Show full text]
  • EE1.El3 (EEE1023): Electronics III Acoustics Lecture 12 Principles Of
    EE1.el3 (EEE1023): Electronics III Acoustics lecture 12 Principles of sound Dr Philip Jackson www.ee.surrey.ac.uk/Teaching/Courses/ee1.el3 Overview for this semester 1. Introduction to sound 2. Human sound perception 3. Noise measurement 4. Sound wave behaviour 5. Reflections and standing waves 6. Room acoustics 7. Resonators and waveguides 8. Musical acoustics 9. Sound localisation L.1 Introduction to sound • Definition of sound • Vibration of matter { transverse waves { longitudinal waves • Sound wave propagation { plane waves { pure tones { speed of sound L.2 Preparation for Acoustics • What is a sound wave? { look up a definition of sound and its properties • Example of a device for manipulating sound { write down or draw your example { explain how it modifies the sound L.3 Definitions of sound \Sensation caused in the ear by the vibration of the surrounding air or other medium", Oxford En- glish Dictionary \Disturbances in the air caused by vibrations, in- formation on which is transmitted to the brain by the sense of hearing", Chambers Pocket Dictionary \Sound is vibration transmitted through a solid, liquid, or gas; particularly, sound means those vi- brations composed of frequencies capable of being detected by ears", Wikipedia L.4 Vibration of a string Let us consider forces on an element of the vibrating string with tension T and ρL mass per unit length, to derive its equation of motion T y + dy dx dx y ds θ dy x y dx T x x + dx Net vertical force from tension between points x and x + dx: dFY = (T sin θ)x+dx − (T sin θ)x (1) Taylor
    [Show full text]
  • Music 170 Assignment 7 1. a Sinusoidal Plane Wave at 20 Hz
    Music 170 assignment 7 1. A sinusoidal plane wave at 20 Hz. has an SPL of 80 decibels. What is the RMS displacement (in millimeters.) of air (in other words, how far does the air move)? 2. A rectangular vibrating surface one foot long is vibrating at 2000 Hz. Assuming the speed of sound is 1000 feet per second, at what angle off axis should the beam's amplitude drop to zero? 3. How many dB less does a cardioid microphone pick up from an incoming sound 90 degrees (π=2 radians) off-axis, compared to a signal coming in frontally (at the angle of highest gain)? 4. Suppose a sound's SPL is 0 dB (i.e., it's about the threshold of hearing at 1 kHz.) What is the total power that you ear receives? (Assume, a bit generously, that the opening is 1 square centimeter). 5. If light moves at 3 · 108 meters per second, and if a certain color has a wavelength of 500 nanometers (billionths of a meter - it would look green to human eyes), what is the frequency? Would it be audible if it were a sound? [NOTE: I gave the speed of light incorrectly (mixed up the units, ouch!) - we'll accept answers based on either the right speed or the wrong one I first gave.] 6. A speaker one meter from you is paying a tone at 440 Hz. If you move to a position 2 meters away (and then stop moving), at what pitch to you now hear the tone? (Hint: don't think too hard about this one).
    [Show full text]
  • Anharmonic Waves in Quantum Electrodynamics
    Anharmonic Waves in Field Theory F. J. Himpsel Physics Department, University of Wisconsin Madison, Madison WI 53706, USA Abstract This work starts from the premise that sinusoidal plane waves cease to be solutions of field theories when turning on an interaction. A nonlinear interaction term generates harmonics analogous to those observed in nonlinear optical media. This calls for a generalization to anharmonic waves in both classical and quantum field theory. Three simple requirements make anharmonic waves compatible with relativistic field theory and quantum physics. Some non-essential concepts have to be abandoned, such as orthogonality, the superposition principle, and the existence of single-particle energy eigenstates. The most general class of anharmonic waves allows for a zero frequency term in the Fourier series, which corresponds to a quantum field with a non-zero vacuum expectation value. Anharmonic quantum fields are defined by generalizing the expansion of a field operator into creation and annihilation operators. This method provides a framework for handling exact quantum fields, which define exact single particle states. ____________________________________ Electronic address: [email protected] 1 Contents 1. General Concept 3 2. Criteria for Anharmonic Waves 5 3. Fourier Series of Anharmonic Waves 6 4. Symmetry Classes 8 5. Energy and Momentum 10 6. Orthonormality and Completeness 12 7. Anharmonic Quantum Fields 13 8. Conclusions and Outlook 16 Appendix A: Fourier Coefficients and Anharmonicity Parameter 17 Appendix B: Expansion of Sinusoidal Waves into Anharmonic Waves 19 Appendix C: Simple Anharmonic Waves 20 Appendix D: Anharmonic Waves from Elliptic Functions 22 Appendix E: Anharmonic Waves from Differential Equations and Lagrangians 25 References 28 2 1.
    [Show full text]
  • Wave Equation
    UNIVERSITY OF OSLO INF5410 Array signal processing. Chapter 2.1-2.2: Wave equation Sverre Holm DEPARTMENT OF INFORMATICS UNIVERSITY OF OSLO Chapters in Johnson & Dungeon • Ch. 1: Introduction . • Ch. 2: Signals in Space and Time. – Physics: Waves and wave equation. »c, λ, f, ω, k vector,... » Ideal and ”real'' conditions • Ch. 3: Apertures and Arrays. • Ch4BCh. 4: Beam form ing. – Classical, time and frequency domain algorithms. • Ch. 7: Adaptive Array Processing. DEPARTMENT OF INFORMATICS 2 1 UNIVERSITY OF OSLO Norsk terminologi • Bølgeligningen • Planbølger, sfæriske bølger • Propagerende bølger, bølgetall • Sinking/sakking: • Dispersjon • Attenuasjon eller demping • Refraksjon • Ikke-linearitet • Diffraksjon; nærfelt, fjernfelt • Gruppeantenne ( = array) Kilde: Bl.a. J. M. Hovem: ``Marin akustikk'', NTNU, 1999 DEPARTMENT OF INFORMATICS 3 UNIVERSITY OF OSLO Wave equation • This is the equation in array signal processing. • Lossless wave equation • Δ=∇2 is the Laplacian operator (del=nabla squared) • s = s(x,y,z,t) is a general scalar field (electromagnetics: electric or magnetic field, acoustics: sound pressure ...) • c is the speed of propagation DEPARTMENT OF INFORMATICS 4 2 UNIVERSITY OF OSLO Three simple principles behind the acoustic wave equation dz 1. Equation of continuity: ∂(ρu& x ) ρu& x + dx conservation of mass ∂x ρu& x 2. Newton’s 2. law: F = m a 3. State equation: relationship between change in pressure and z dy volume (in one dimension this y dx is Hooke’s law: F = k x – spring) x Figure: J Hovem, TTT4175 Marin akustikk,
    [Show full text]
  • DESIGN of DIFFRACTIVE OPTICAL ELEMENTS: OPTIMALITY, SCALE and NEAR-FIELD DIFFRACTION CONSIDERATIONS Parker Kuhl
    Purdue University Purdue e-Pubs ECE Technical Reports Electrical and Computer Engineering 1-1-2003 DESIGN OF DIFFRACTIVE OPTICAL ELEMENTS: OPTIMALITY, SCALE AND NEAR-FIELD DIFFRACTION CONSIDERATIONS Parker Kuhl Okan K. Ersoy Follow this and additional works at: http://docs.lib.purdue.edu/ecetr Kuhl, Parker and Ersoy, Okan K. , "DESIGN OF DIFFRACTIVE OPTICAL ELEMENTS: OPTIMALITY, SCALE AND NEAR- FIELD DIFFRACTION CONSIDERATIONS" (2003). ECE Technical Reports. Paper 151. http://docs.lib.purdue.edu/ecetr/151 This document has been made available through Purdue e-Pubs, a service of the Purdue University Libraries. Please contact [email protected] for additional information. DESIGN OF DIFFRACTIVE OPTICAL ELEMENTS: OPTIMALITY, SCALE AND NEAR-FIELD DIFFRACTION CONSIDERATIONS Parker Kuhl Okan K. Ersoy TR-ECE 03-09 School of Electrical and Computer Engineering 465 Northwestern Avenue Purdue University West Lafayette, IN 47907-2035 ii iii TABLE OF CONTENTS LIST OF TABLES .............................................................................................................v LIST OF FIGURES ........................................................................................................ vii ABSTRACT.......................................................................................................................ix 1 INTRODUCTION......................................................................................................... 1 2. DIFFRACTION ..........................................................................................................
    [Show full text]
  • Chapter 7. Electromagnetic Wave Propagation
    Essential Graduate Physics EM: Classical Electrodynamics Chapter 7. Electromagnetic Wave Propagation This (rather extensive) chapter focuses on the most important effect that follows from the time- dependent Maxwell equations, namely the electromagnetic waves, at this stage avoiding a discussion of their origin, i.e. the radiation process – which will the subject of Chapters 8 and 10. The discussion starts from the simplest, plane waves in uniform and isotropic media, and then proceeds to non-uniform systems, bringing up such effects as reflection and refraction. Then we will discuss the so-called guided waves, propagating along various long transmission lines – such as coaxial cables, waveguides, and optical fibers. Finally, the end of the chapter is devoted to final-length fragments of such lines, serving as resonators, and to effects of energy dissipation in transmission lines and resonators. 7.1. Plane waves Let us start from considering a spatial region that does not contain field sources ( = 0, j = 0), and is filled with a linear, uniform, isotropic medium, which obeys Eqs. (3.46) and (5.110): D E,B H . (7.1) Moreover, let us assume for a while, that these constitutive equations hold for all frequencies of interest. (Of course, these relations are exactly valid for the very important particular case of free space, where we may formally use the macroscopic Maxwell equations (6.100), but with = 0 and = 0.) As was already shown in Sec. 6.8, in this case, the Lorenz gauge condition (6.117) allows the Maxwell equations to be recast into the wave equations (6.118) for the scalar and vector potentials.
    [Show full text]
  • Plane Wave Propagation in Lossless Media See Animation “Plane Wave Viewer” 1 Plane Waves in Lossless Media in a Source Free Lossless Medium, J = Ρ = Σ = 0
    NUS/ECE EE2011 Plane Wave Propagation in Lossless Media See animation “Plane Wave Viewer” 1 Plane Waves in Lossless Media In a source free lossless medium, J = ρ = σ = 0. Maxwell’s equations: J =current density ρ =charge density ∂H ∇× E = -μ σ =conductivity ∂t ∂E ∇× H = ε ∂t ε∇ ⋅E = 0 μ∇ ⋅ H = 0 Hon Tat Hui 1 Plane Wave Propagation in Lossless Media NUS/ECE EE2011 Take the curl of the first equation and make use of the second and the third equations, we have: Note : ∇×∇×E = ∇()∇ ⋅E − ∇2E ∂ ∂ 2 ∇ 2E = μ ∇× H = με E ∂t ∂t 2 This is called the wave equation: ∂2 ∇2E − με E = 0 ∂t 2 A similar equation for H can be obtained: ∂2 ∇2H − με H = 0 ∂t 2 Hon Tat Hui 2 Plane Wave Propagation in Lossless Media NUS/ECE EE2011 In free space, the wave equation for E is: ∂ 2 ∇ 2E − μ ε E = 0 0 0 ∂t 2 where 1 μ ε = 0 0 c2 c being the speed of light in free space (~ 3 × 108 (m/s)). Hence the speed of light can be derived from Maxwell’s equation. Hon Tat Hui 3 Plane Wave Propagation in Lossless Media Signal Propagation - 시간 지연 - 시간영역 파형 유지 Ef(0)= (t ) Ef()r= ( t − rc / ) NUS/ECE EE2011 To simplify subsequent analyses, we consider a special case in which the field (and the source) variation with time takes the form of a sinusoidal function: sin(ωt +φ) or cos(ωt +φ) Using complex notation, the E field, for example, can be written as: • ⎧ jωt ⎫ E()x, y, z,t = Re⎨E ()x, y, z e ⎬ ⎩ ⎭ • where E () x , y , z is called the phasor form of E(x,y,z,t) and is in general a complex number depending on the spatial coordinates only.
    [Show full text]
  • Lecture 7 More on Constitute Relations, Uniform Plane Wave
    Lecture 7 More on Constitute Relations, Uniform Plane Wave 7.1 More on Constitutive Relations As have been seen, Maxwell's equations are not solvable until the constitutive relations are included. Here, we will look into depth more into various kinds of constitutive relations. 7.1.1 Isotropic Frequency Dispersive Media First let us look at the simple linear constitutive relation previously discussed for dielectric media where [29], [31][p. 82], [42] D = "0E + P (7.1.1) We have a simple model where P = "0χ0E (7.1.2) where χ0 is the electric susceptibility. When used in the generalized Ampere's law, P, the polarization density, plays an important role for the flow of the displacement current through space. The polarization density is due to the presence of polar atoms or molecules that become little dipoles in the presence of an electric field. For instance, water, which is H2O, is a polar molecule that becomes a small dipole when an electric field is applied. We can think of displacement current flow as capacitive coupling yielding polarization current flow through space. Namely, for a source-free medium, @D @E @P r × H = = " + (7.1.3) @t 0 @t @t 63 64 Electromagnetic Field Theory Figure 7.1: As a series of dipoles line up end to end, one can see a current flowing through the line of dipoles as they oscillate back and forth in their polarity. This is similar to how displacement current flows through a capacitor. For example, for a sinusoidal oscillating field, the dipoles will flip back and forth giving rise to flow of displacement current just as how time-harmonic electric current can flow through a capacitor as shown in Figure 7.1.
    [Show full text]
  • Physics 380H - Wave Theory Homework #03 Fall 2004 Due 12:01 PM, Monday 2004/10/04
    Physics 380H - Wave Theory Homework #03 Fall 2004 Due 12:01 PM, Monday 2004/10/04 [50 points total] “Journal” questions: – Considering your entire history as a student, what course (in any subject) has been the most rewarding for you? Why? – Any comments about this week’s activities? Course content? Assignment? Lab? 1. (From Towne P2-6. pg 36) Show from the basic equations of the acoustic approximation that p, s, ξ, and ξ˙ all satisfy the one-dimensional wave equation. [10] 2. (From Towne P2-10. pg 36) Consider a progressive sinusoidal plane wave of given frequency ω and displacement amplitude ξm travelling in air, and a wave having the same values of ω and ξm traveling in water. How do the pressure amplitudes compare? If the value of sm for the wave in water is sufficiently small to satisfy the acoustic approximation, is it necessarily so for the wave in air?. [10] 3. (From Towne P2-20. pg 38) Determination of an acoustic wave from given initial conditions: (a) For plane waves satisfying the linearized one-dimensional wave equation in a uniform fluid medium of infinite extent, assume that the function ξ˙(x, 0), which specifies the initial velocities of all the particles, and the initial pressure distribution, p(x, 0), are given. Find the general expression for p(x, t). [10] (b) Apply your general result from part (a) to the special case of particles initially at rest, p , x < 0, p(x, 0) = 0 0, x ≥ 0. Plot or sketch the graph of p(x, t) at some later time.
    [Show full text]
  • ECE 604, Lecture 7
    ECE 604, Lecture 7 Jan 23, 2019 Contents 1 More on Constitutive Relations 2 1.1 Isotropic Frequency Dispersive Media . 2 1.2 Anisotropic Media . 3 1.3 Bi-anisotropic Media . 4 1.4 Inhomogeneous Media . 4 1.5 Uniaxial and Biaxial Media . 4 1.6 Nonlinear Media . 5 2 Wave Phenomenon in the Frequency Domain 5 3 Uniform Plane Waves in 3D 6 Printed on March 24, 2019 at 16 : 05: W.C. Chew and D. Jiao. 1 ECE 604, Lecture 7 Jan 23, 2019 1 More on Constitutive Relations 1.1 Isotropic Frequency Dispersive Media First let us look at the simple constitutive relation for the where D = "0E + P (1.1) We have a simple model where P = "0χ0E (1.2) where χ0 is the electric susceptibility. When used in the generalized Ampere's law, P, the polarization density, plays an important role for the flow of the displacement current through space. The polarization density can be due to the presence of polar atoms or molecules that become little dipoles in the presence of an electric field. For instance, water, which is H2O, is a polar molecule that becomes a small dipole when an electric field is applied. We can think of displacement current flow as capacitive coupling of polar- ization current flow through space. Namely, for a source-free medium, @D @E @P r × H = = " + (1.3) @t 0 @t @t Figure 1: For example, for a sinusoidal oscillating field, the dipoles will flip back and forth giving rise to flow of displacement current just as how time-harmonic electric current can flow through a capacitor as shown in Figure 1.
    [Show full text]
  • Lecture 7 More on Constitute Relations, Uniform Plane Wave
    Lecture 7 More on Constitute Relations, Uniform Plane Wave 7.1 More on Constitutive Relations As have been seen, Maxwell's equations are not solvable until the constitutive relations are included. Here, we will look into depth more into various kinds of constitutive relations. Now that we have learned phasor technique, we can have a more general constitutive relationship compared to what we have seen earlier. 7.1.1 Isotropic Frequency Dispersive Media First let us look at the simple linear constitutive relation previously discussed for dielectric media where [30], [31][p. 82], [43] D = "0E + P (7.1.1) We have a simple model where P = "0χ0E (7.1.2) where χ0 is the electric susceptibility. When used in the generalized Ampere's law, P, the polarization density, plays an important role for the flow of the displacement current through space. The polarization density is due to the presence of polar atoms or molecules that become little dipoles in the presence of an electric field. For instance, water, which is H2O, is a polar molecule that becomes a small dipole when an electric field is applied. We can think of displacement current flow as capacitive coupling yielding polarization current flow through space. Namely, for a source-free medium, @D @E @P r × H = = " + (7.1.3) @t 0 @t @t 61 62 Electromagnetic Field Theory Figure 7.1: As a series of dipoles line up end to end, one can see a current flowing through the line of dipoles as they oscillate back and forth in their polarity. This is similar to how displacement current flows through a capacitor.
    [Show full text]