Plane Waves, Polarization and the Poynting Vector

Total Page:16

File Type:pdf, Size:1020Kb

Plane Waves, Polarization and the Poynting Vector Plane Waves, Polarization and the Poynting Vector EE H =-xx+- y hh Uniform Plane Wave in Free Space We have previously established the following properties of plane waves in free space: • Electric and magnetic field components in propagation direction are zero. rr rr • Electric and magnetic fields (EBxy, or EByx, ) are related. Each is the “source” of the other. • A set of three second order differential equations apply, one for each field component in rectangular coordinates. For example: rr ∂ 2 E me∂2 E xoox= , ∂ z 2 ∂t 2 or for harmonic fields, in phasor notation: r ∂ 2E r x =-wme2 E ∂ z 2 oo x A general solution to the Helmholz equation is written: r rrr - jzbboo jz ECx =+12ee C (C i can be complex), where bwmewooo==/c, c = speed of light. Propagation of Magnetic Field Suppose we haverr an electric field wave travelling in the positive z direction. Recall that curl EB=-jw , or for our travelling wave, r rr r - jzb ∂ E EE= e o x xxo+ =-jw B y r ∂ z - jzb o r ∂ diE + xo e =-jw B ∂ z y rrrb -=-fi=jebwEBBE- jzbbo jo e- jzo oxo+ yyw + xo w r = E e - jzb o cw + xo r • Electric and magnetic (B ) field are orthogonal (perpendicular, Right Hand Rule), in-phase, and the ratio of the field magnitudes is the imped- ance. It isr very useful to expressr this ratio of electric and magnetic fields in terms of H , rather than B . r r E r mmeH ==x E , oy c xoo r Er x m o m o or, after rearranging: ==m o c = H y emoo e o Henry/ m Joule/ amp 2 volt Dimensional analysis: ===Ohm!!! Farad/ m Joule/ volt 2 amp or: r Electric fields are volts/meter and H fields are amps/meter. r Er x m o =∫ho Ohms, hpo ª=120 377 Ohmsr (impedance of freespace) H y e o $ Er x For a wave travelling in the - ez direction, =-ho . This just means that r H r $ y E x is oriented along the - ex direction (or equivalently with H y ). Summary: r r •E and H are perpendicular to each other and propagation direction. Right Hand Rule gives direction. r r • Ratio of H to E is the intrinsic wave impedance, ho . The wavelength is the distance that the wave travels so that the phase changes by 2p radi- ans. 222p p pcc blo = 2 p, or l == = = bo w/c w f •Picture: • Phase velocity, vp To understand the phase velocity, we must return to the real representation of the field with both space and time dependence; that is, EE=-+ xocosbgwb t o z Consider an observer moving along in z at the same point, say the peak, of the oscillating field. This means mathematically that: wbtz-=o 0 or any constant. Thus, wbdt= o dz , dz w or =∫vp , the phase velocity. dt bo Polarization of Place Waves Consider the propagation characteristics of a plane wave in which the elec- tric field has components in both the x and y directions: rr r $$- jzb o , EE=+dixxeee E yy where the field components may be complex. That is, rr rr ja jb EExx= e and EEyy= e In phase ab= , rr r jza $$--bgb o EE=+ejxxeee E yy or in real form: rr r EEeEe=+e xx yyj cosbgwb t -- o za y r Ey r E r x Ex z This is linear polarization. Now we consider a more general case. Elliptical Polarization In this case we allow arbitrary phase relationships a and b: rr r ja jb - jzb o EE=+ejeexxeeeyy E It is easier to see what this means if we write each component out in real form: rr EE=+-cosafwb taz rrxx EEyy=+-cosafwb tbz Suppose we let a = 0 and b = p /2. Then: rr EExx=-cosafwb tz rr EEyy=-sin afwb tz - rrr What can we say about Eztaf, =+ Exxee E yy? rr1 Make a plot in the x-y plane with t as a parameter and EE==1, . xy2 r r wt E x Ey 0 1 1 0 5 6 7 .707p /4 2 −./707 2 1 p/2 3 0 − 12/ 4 − 2 p 4 1 0 3 54p/ 5 −.707 ./707 2 32p / 6 0 12/ 74.707p/ 7 ./707 2 This clockwise rotation describes an ellipse, with major axes parallel to the x axis. As the wave propagates along z, the ellipse spreads out to anrr elliptical helix. This is called elliptical polarization. For the special case of EExy= , we have circular polarization. If we had chosen b =-p /2, we would have found that an identical ellipse would be formed except that the rotation would be counter-clockwise. Poynting Theorem We know that energy is propagated by waves, in general, and electromag- netic waves, in particular. We need to quantify the associated power flow. We easily obtain a hint of how to calculate power flow by recalling our circuit theory, where PVI= * , or by a dimensional analysis of the fields. Remember that the units of H are Amp/meter and the units of E are V/m. Their product Amp Volts/m2 has units of Watts/area, which is a power den- sity, just what we want. The product must clearly have a direction associ- ated with it, and it ought to somehow point in a reasonable direction. A reasonable direction for power flow in lossless, homogeneous, linear media, such as free space, wouldrr be in the direction of propagation. We might therefore guess that EH¥ would be a reasonable definition of power den- sity. We will consider the complex Poynting vector for time harmonic plane elec- tromagnetic waves in phasor notation. This requires some thought because rr of the nonlinear nature of EH¥ . r r jtw $ Let Eztaf, = Re E af ze ex and r r jt w $ Hztaf, = Re H af ze ey We will write out the real and imaginary parts of E and H. r rr jtwwjt $ Ezta, f=+Re EEr af ze ji af ze ex and r rr jtwwjt $ Hztaf, =+Re HHr af ze ji af ze ey Now expand the complex exponential and take the real part: rr r $ Ezta,cossin f=- Erix af zww t Ez af te rr r $ Hzta,cossin f=- Hriy af zww t Hz af te rrr The Poynting vector is: Pztaf, =¥ E H = rr rr rr rr 22 $ EHrrcoswwwwww t+- EH ii sin t EH ri cos t sin t - EH ir sin t cos te z The time average Poynting vector is: rr rrrr 11T 1 Pzav af==+Pztdt a, f EHrr EH ii T z0 2 2 The very same expression can be obtained directly from the phasors by the following rule: r rr r r r r 1 1 $$ Pztaf,*=¥=+¥-RediEH Re d Erixriy j E idi e H j H e 2 2 rr rr 1 $ =+diEHrr EH iiz e 2 Example What is the time average Poynting vector for a plane wave propagating in free space with the following (phasor) fields: r r E+0 - jzb o - jzb o $ H afz = ee$ E afzEee= +0 x and y ? h o r 1 rr Then Pztav af, =¥=RediEH* 2 1 F E I 1 E 2 - jzbboo$$+00- jz + $, ReG Ee+0 ex ¥ eey J = Re ez 2 H hho K 2 o or: r E 2 +0 $ Pztav af, = ez 2ho.
Recommended publications
  • Lab 8: Polarization of Light
    Lab 8: Polarization of Light 1 Introduction Refer to Appendix D for photos of the appara- tus Polarization is a fundamental property of light and a very important concept of physical optics. Not all sources of light are polarized; for instance, light from an ordinary light bulb is not polarized. In addition to unpolarized light, there is partially polarized light and totally polarized light. Light from a rainbow, reflected sunlight, and coherent laser light are examples of po- larized light. There are three di®erent types of po- larization states: linear, circular and elliptical. Each of these commonly encountered states is characterized Figure 1: (a)Oscillation of E vector, (b)An electromagnetic by a di®ering motion of the electric ¯eld vector with ¯eld. respect to the direction of propagation of the light wave. It is useful to be able to di®erentiate between 2 Background the di®erent types of polarization. Some common de- vices for measuring polarization are linear polarizers and retarders. Polaroid sunglasses are examples of po- Light is a transverse electromagnetic wave. Its prop- larizers. They block certain radiations such as glare agation can therefore be explained by recalling the from reflected sunlight. Polarizers are useful in ob- properties of transverse waves. Picture a transverse taining and analyzing linear polarization. Retarders wave as traced by a point that oscillates sinusoidally (also called wave plates) can alter the type of polar- in a plane, such that the direction of oscillation is ization and/or rotate its direction. They are used in perpendicular to the direction of propagation of the controlling and analyzing polarization states.
    [Show full text]
  • Chapter 3 Electromagnetic Waves & Maxwell's Equations
    Chapter 3 Electromagnetic Waves & Maxwell’s Equations Part I Maxwell’s Equations Maxwell (13 June 1831 – 5 November 1879) was a Scottish physicist. Famous equations published in 1861 Maxwell’s Equations: Integral Form Gauss's law Gauss's law for magnetism Faraday's law of induction (Maxwell–Faraday equation) Ampère's law (with Maxwell's addition) Maxwell’s Equations Relation of the speed of light and electric and magnetic vacuum constants 1 c = 2.99792458 108 [m/s] 0 0 permittivity of free space, also called the electric constant permeability of free space, also called the magnetic constant Gauss’s Law For any closed surface enclosing total charge Qin, the net electric flux through the surface is This result for the electric flux is known as Gauss’s Law. Magnetic Gauss’s Law The net magnetic flux through any closed surface is equal to zero: As of today there is no evidence of magnetic monopoles See: Phys.Rev.Lett.85:5292,2000 Ampère's Law The magnetic field in space around an electric current is proportional to the electric current which serves as its source: B ds 0I I is the total current inside the loop. ds B i1 Direction of integration i 3 i2 Faraday’s Law The change of magnetic flux in a loop will induce emf, i.e., electric field B E ds dA A t Lenz's Law Claim: Direction of induced current must be so as to oppose the change; otherwise conservation of energy would be violated. Problem with Ampère's Law Maxwell realized that Ampere’s law is not valid when the current is discontinuous.
    [Show full text]
  • Observation of Elliptically Polarized Light from Total Internal Reflection in Bubbles
    Observation of elliptically polarized light from total internal reflection in bubbles Item Type Article Authors Miller, Sawyer; Ding, Yitian; Jiang, Linan; Tu, Xingzhou; Pau, Stanley Citation Miller, S., Ding, Y., Jiang, L. et al. Observation of elliptically polarized light from total internal reflection in bubbles. Sci Rep 10, 8725 (2020). https://doi.org/10.1038/s41598-020-65410-5 DOI 10.1038/s41598-020-65410-5 Publisher NATURE PUBLISHING GROUP Journal SCIENTIFIC REPORTS Rights Copyright © The Author(s) 2020. Open Access This article is licensed under a Creative Commons Attribution 4.0 International License. Download date 29/09/2021 02:08:57 Item License https://creativecommons.org/licenses/by/4.0/ Version Final published version Link to Item http://hdl.handle.net/10150/641865 www.nature.com/scientificreports OPEN Observation of elliptically polarized light from total internal refection in bubbles Sawyer Miller1,2 ✉ , Yitian Ding1,2, Linan Jiang1, Xingzhou Tu1 & Stanley Pau1 ✉ Bubbles are ubiquitous in the natural environment, where diferent substances and phases of the same substance forms globules due to diferences in pressure and surface tension. Total internal refection occurs at the interface of a bubble, where light travels from the higher refractive index material outside a bubble to the lower index material inside a bubble at appropriate angles of incidence, which can lead to a phase shift in the refected light. Linearly polarized skylight can be converted to elliptically polarized light with efciency up to 53% by single scattering from the water-air interface. Total internal refection from air bubble in water is one of the few sources of elliptical polarization in the natural world.
    [Show full text]
  • Poynting Vector and Power Flow in Electromagnetic Fields
    Poynting Vector and Power Flow in Electromagnetic Fields: Electromagnetic waves can transport energy as a result of their travelling or propagating characteristics. Starting from Maxwell's Equations: Together with the vector identity One can write In simple medium where and are constant, and Divergence theorem states, This equation is referred to as Poynting theorem and it states that the net power flowing out of a given volume is equal to the time rate of decrease in the energy stored within the volume minus the conduction losses. In the equation, the following term represents the rate of change of the stored energy in the electric and magnetic fields On the other hand, the power dissipation within the volume appears in the following form Hence the total decrease in power within the volume under consideration: Here (W/mt2) is called the Poynting vector and it represents the power density vector associated with the electromagnetic field. The integration of the Poynting vector over any closed surface gives the net power flowing out of the surface. Poynting vector for the time harmonic case: Using the convention, the instantaneous value of a quantity is the real part of the product of a phasor quantity and when is used as reference. Considering the following phasor: −푗훽푧 퐸⃗ (푧) = 푥̂퐸푥(푧) = 푥̂퐸0푒 The instantaneous field becomes: 푗푤푡 퐸⃗ (푧, 푡) = 푅푒{퐸⃗ (푧)푒 } = 푥̂퐸0푐표푠(휔푡 − 훽푧) when E0 is real. Let us consider two instantaneous quantities A and B such that where A and B are the phasor quantities. Therefore, Since A and B are periodic with period , the time average value of the product form AB, 푇 1 퐴퐵 = ∫ 퐴퐵푑푡 푎푣푒푟푎푔푒 푇 0 푇 1 퐴퐵 = ∫|퐴||퐵|푐표푠(휔푡 + 훼)푐표푠(휔푡 + 훽)푑푡 푎푣푒푟푎푔푒 푇 0 1 퐴퐵 = |퐴||퐵|푐표푠(훼 − 훽) 푎푣푒푟푎푔푒 2 For phasors, and , where * denotes complex conjugate.
    [Show full text]
  • Electromagnetic Energy
    Physics 142 Electromagnetic Enmergy Page !1 Electromagnetic Energy A child of five can understand this; send someone to fetch a child of five. — Groucho Marx Energy in the fields can move from place to place We have discussed the energy in an electrostatic field, such as that stored in a capacitor. We found that this energy can be thought of as distributed in space, with an energy per unit volume (energy density) at each point in space. We obtained a formula for this 1 2 quantity, ! ue = 2 ε0E (if there are no dielectric materials). This formula applies to any E- field. We also found that magnetic fields possess energy distributed in space, described 2 by the magnetic energy density ! um = B /2µ0 . If there are both electric and magnetic fields, the total electromagnetic energy density is the sum of ! ue and ! um . These specify how much electromagnetic field energy there is at any point in space. But we have not yet considered how this energy moves from place to place. Consider the energy flow in a flashlight. We know that energy moves from the battery to the bulb, where it is converted into heat and light. It is tempting to assume that this energy flows through the conductors, like water in a pipe. But if we look carefully we find that the electromagnetic energy density in the conductors is much too small to account for the amount of energy in transit. Nearly all of the energy gets to the bulb by flowing through space near the conductors. In a sense they guide the energy but do not carry much of it.
    [Show full text]
  • Ellipsometry
    AALBORG UNIVERSITY Institute of Physics and Nanotechnology Pontoppidanstræde 103 - 9220 Aalborg Øst - Telephone 96 35 92 15 TITLE: Ellipsometry SYNOPSIS: This project concerns measurement of the re- fractive index of various materials and mea- PROJECT PERIOD: surement of the thickness of thin films on sili- September 1st - December 21st 2004 con substrates by use of ellipsometry. The el- lipsometer used in the experiments is the SE 850 photometric rotating analyzer ellipsome- ter from Sentech. THEME: After an introduction to ellipsometry and a Detection of Nanostructures problem description, the subjects of polar- ization and essential ellipsometry theory are covered. PROJECT GROUP: The index of refraction for silicon, alu- 116 minum, copper and silver are modelled us- ing the Drude-Lorentz harmonic oscillator model and afterwards measured by ellipsom- etry. The results based on the measurements GROUP MEMBERS: show a tendency towards, but are not ade- Jesper Jung quately close to, the table values. The mate- Jakob Bork rials are therefore modelled with a thin layer of oxide, and the refractive indexes are com- Tobias Holmgaard puted. This model yields good results for the Niels Anker Kortbek refractive index of silicon and copper. For aluminum the result is improved whereas the result for silver is not. SUPERVISOR: The thickness of a thin film of SiO2 on a sub- strate of silicon is measured by use of ellip- Kjeld Pedersen sometry. The result is 22.9 nm which deviates from the provided information by 6.5 %. The thickness of two thick (multiple wave- NUMBERS PRINTED: 7 lengths) thin polymer films are measured. The polymer films have been spin coated on REPORT PAGE NUMBER: 70 substrates of silicon and the uniformities of the surfaces are investigated.
    [Show full text]
  • Poynting's Theorem and the Wave Equation
    Chapter 18: Poynting’s Theorem and the Wave Equation Chapter Learning Objectives: After completing this chapter the student will be able to: Use Poynting’s theorem to determine the direction and magnitude of power flow in an electromagnetic system. Use Maxwell’s Equations to derive a general homogeneous wave equation for the electric and magnetic field. Derive a simplified wave equation assuming propagation in a vacuum and an electric field polarized in only one direction. Use Maxwell’s Equations to derive the speed of light in a vacuum. You can watch the video associated with this chapter at the following link: Historical Perspective: John Henry Poynting (1852-1914) was an English physicist who did work in electromagnetic energy flow, elasticity, and astronomy. He coined the term “Greenhouse Effect.” Both the Poynting Vector and Poynting’s Theorem are named in his honor. Photo credit: https://upload.wikimedia.org/wikipedia/commons/5/5f/John_Henry_Poynting.jpg, [Public domain], via Wikimedia Commons. 1 18.1 Poynting’s Theorem With Maxwell’s Equations, we now have the tools necessary to derive Poynting’s Theorem, which will allow us to perform many useful calculations involving the direction of power flow in electromagnetic fields. We will begin with Faraday’s Law, and we will take the dot product of H with both sides: (Copy of Equation 16.24) (Equation 18.1) Next, we will start with Ampere’s Law and will take the dot product of E with both sides: (Copy of Equation 17.13) (Equation 18.2) Now, let’s subtract both sides of Equation 18.2 from both sides of Equation 18.1: (Equation 18.3) We can now apply the following mathematical identity to the left side of Equation 18.3: (Equation 18.4) This substitution yields: (Equation 18.5) Distributing the E across the right side gives: (Equation 18.6) 2 Now let’s concentrate on the first time on the right side.
    [Show full text]
  • Understanding Polarization
    Semrock Technical Note Series: Understanding Polarization The Standard in Optical Filters for Biotech & Analytical Instrumentation Understanding Polarization 1. Introduction Polarization is a fundamental property of light. While many optical applications are based on systems that are “blind” to polarization, a very large number are not. Some applications rely directly on polarization as a key measurement variable, such as those based on how much an object depolarizes or rotates a polarized probe beam. For other applications, variations due to polarization are a source of noise, and thus throughout the system light must maintain a fixed state of polarization – or remain completely depolarized – to eliminate these variations. And for applications based on interference of non-parallel light beams, polarization greatly impacts contrast. As a result, for a large number of applications control of polarization is just as critical as control of ray propagation, diffraction, or the spectrum of the light. Yet despite its importance, polarization is often considered a more esoteric property of light that is not so well understood. In this article our aim is to answer some basic questions about the polarization of light, including: what polarization is and how it is described, how it is controlled by optical components, and when it matters in optical systems. 2. A description of the polarization of light To understand the polarization of light, we must first recognize that light can be described as a classical wave. The most basic parameters that describe any wave are the amplitude and the wavelength. For example, the amplitude of a wave represents the longitudinal displacement of air molecules for a sound wave traveling through the air, or the transverse displacement of a string or water molecules for a wave on a guitar string or on the surface of a pond, respectively.
    [Show full text]
  • The Poynting Vector: Power and Energy in Electromagnetic fields
    The Poynting vector: power and energy in electromagnetic fields Kenneth H. Carpenter Department of Electrical and Computer Engineering Kansas State University October 19, 2004 1 Conservation of energy in electromagnetics The concept of conservation of energy (along with conservation of momen- tum) is one of the basic principles of physics – both classical and modern. When dealing with electromagnetic fields a way is needed to relate the con- cept of energy to the fields. This is done by means of the Poynting vector: P = E × H. (1) In eq.(1) E is the electric field intensity, H is the magnetic field intensity, and P is the Poynting vector, which is found to be the power density in the electromagnetic field. The conservation of energy is then established by means of the Poynting theorem. 2 The Poynting theorem By using the Maxwell equations for the curl of the fields along with Gauss’s divergence theorem and an identity from vector analysis, we may prove what is known as the Poynting theorem. 1 EECE557 Poynting vector – supplement to text - Fall 2004 2 The Maxwell’s equations needed are ∂B ∇ × E = − (2) ∂t ∂D ∇ × H = J + (3) ∂t along with the material relationships D = 0E + P (4) B = µ0H + µ0M (5) or for isotropic materials D = E (6) B = µH (7) In addition, the identity from vector analysis, ∇ · (E × H) ≡ −E · (∇ × H) + H · (∇ × E), (8) is needed. 2.1 The derivation If P is to be power density, then its surface integral over the surface of a volume must be the power out of the volume.
    [Show full text]
  • PHYS 110B - HW #4 Fall 2005, Solutions by David Pace Equations Referenced As ”EQ
    PHYS 110B - HW #4 Fall 2005, Solutions by David Pace Equations referenced as ”EQ. #” are from Griffiths Problem statements are paraphrased [1.] Problem 8.2 from Griffiths Reference problem 7.31 (figure 7.43). (a) Let the charge on the ends of the wire be zero at t = 0. Find the electric and magnetic fields in the gap, E~ (s, t) and B~ (s, t). (b) Find the energy density and Poynting vector in the gap. Verify equation 8.14. (c) Solve for the total energy in the gap; it will be time-dependent. Find the total power flowing into the gap by integrating the Poynting vector over the relevant surface. Verify that the input power is equivalent to the rate of increasing energy in the gap. (Griffiths Hint: This verification amounts to proving the validity of equation 8.9 in the case where W = 0.) Solution (a) The electric field between the plates of a parallel plate capacitor is known to be (see example 2.5 in Griffiths), σ E~ = zˆ (1) o where I define zˆ as the direction in which the current is flowing. We may assume that the charge is always spread uniformly over the surfaces of the wire. The resultant charge density on each “plate” is then time-dependent because the flowing current causes charge to pile up. At time zero there is no charge on the plates, so we know that the charge density increases linearly as time progresses. It σ(t) = (2) πa2 where a is the radius of the wire and It is the total charge on the plates at any instant (current is in units of Coulombs/second, so the total charge on the end plate is the current multiplied by the length of time over which the current has been flowing).
    [Show full text]
  • PHYS 332 Homework #1 Maxwell's Equations, Poynting Vector, Stress
    PHYS 332 Homework #1 Maxwell's Equations, Poynting Vector, Stress Energy Tensor, Electromagnetic Momentum, and Angular Momentum 1 : Wangsness 21-1. A parallel plate capacitor consists of two circular plates of area S (an effectively infinite area) with a vacuum between them. It is connected to a battery of constant emf . The plates are then slowly oscillated so that the separation d between ~ them is described by d = d0 + d1 sin !t. Find the magnetic field H between the plates produced by the displacement current. Similarly, find H~ if the capacitor is first disconnected from the battery and then the plates are oscillated in the same manner. 2 : Wangsness 21-7. Find the form of Maxwell's equations in terms of E~ and B~ for a linear isotropic but non-homogeneous medium. Do not assume that Ohm's Law is valid. 3 : Wangsness 21-9. Figure 21-3 shows a charging parallel plate capacitor. The plates are circular with radius a (effectively infinite). Find the Poynting vector on the bounding surface of region 1 of the figure. Find the total rate at which energy is entering region 1 and then show that it equals the rate at which the energy of the capacitor is increasing. 4a: Extra-2. You have a parallel plate capacitor (assumed infinite) with charge densities σ and −σ and plate separation d. The capacitor moves with velocity v in a direction perpendicular to the area of the plates (NOT perpendicular to the area vector for the plates). Determine S~. b: This time the capacitor moves with velocity v parallel to the area of the plates.
    [Show full text]
  • Lecture 16 Waves in Isotropic Media: Dielectrics And
    Lecture 16 Waves in Isotropic Media: Dielectrics and Conductors In this lecture you will learn: • Wave propagation in dielectric media • Waves propagation in conductive media ECE 303 – Fall 2005 – Farhan Rana – Cornell University Review: Plane Waves in Free Space Faraday’s Law: r r r r ∇ × E()r = − j ω µo H ()r Ampere’s Law: r r r v r r ∇ × H()r = J()r + j ω εo E(r ) r Complex Wave Equation: Assume: J(rv) = ρ(rr) = 0 r r r r 2 r r ∇ × ∇ × E()r = − j ω µo ∇ × H(r ) = ω µo εo E(r ) 0 r r 2 r r 2 r r ⇒ ∇()∇ .E()r − ∇ E()r = ω µo εo E ()r 2 r r 2 r r ⇒ ∇ E()r = −ω µo εo E ()r For a plane wave in free space we know the E-field and H-field phasors to be: r r r r ˆ − j k .r ω E r E()r = n Eo e k = ω µ ε = k o o c r E r r H()rr = kˆ × nˆ o e− j k .r µ ( ) η = o ≈ 377 Ω H ηo o εo ECE 303 – Fall 2005 – Farhan Rana – Cornell University 1 Waves in a Dielectric Medium – Wave Equation Suppose we have a plane wave of the form, E r r r E()rr = nˆ E e− j k .r o ε traveling in an infinite dielectric medium with permittivity ε H What is different from wave propagation in free space? Faraday’s Law: r r r r ∇ × E()r = − j ω µo H ()r Ampere’s Law: r r r ∇ × H()rr = J()rv + j ω ε E(rr) r Complex Wave Equation: Assume: J(rv) = ρ(rr) = 0 r r r r 2 r r compare with the ∇ × ∇ × E()r = − j ω µo ∇ × H(r ) = ω µo ε E(r ) 0 complex wave equation r r 2 r r 2 r r in free space ⇒ ∇()∇ .E()r − ∇ E()r = ω µo ε E ()r 2 r r 2 r r 2 r r 2 r r ⇒ ∇ E()r = −ω µo ε E ()r ∇ E(r )()= −ω µo εo E r ECE 303 – Fall 2005 – Farhan Rana – Cornell University Waves in a Dielectric Medium
    [Show full text]