Plane Electromagnetic Waves

Total Page:16

File Type:pdf, Size:1020Kb

Plane Electromagnetic Waves Plane Electromagnetic Waves EE142 Dr. Ray Kwok •reference: Fundamentals of Engineering Electromagnetics , David K. Cheng (Addison-Wesley) Electromagnetics for Engineers, Fawwaz T. Ulaby (Prentice Hall) Plane EM Wave - Dr. Ray Kwok Source-free Maxwell Equations r r ε∇ ⋅E = ρf r in source-free medium ∇ ⋅ E = 0 r r ∂H (homogeneous, r ∂H ∇× E = −µ linear, isotropic) ∇× E = −µ r ∂t ∂t ρ = 0, J = 0 r ∇ ⋅H = 0 r ∇ ⋅ H = 0 r r r ∂E r ∇× H = J + ε ∂E f ∇× H = ε ∂t ∂t Plane EM Wave - Dr. Ray Kwok Wave Equationr r ∂H ∇ × E = −µ r∂t r ∂E ∇ × H = ε ∂t r r r r 2 ∂H ∂ ∂ E ∇ × ()∇ × E = ∇×− µ = −µ ()∇× H = −µε 2 ∂t ∂t ∂t r r r r ∇ × ()()∇ × E = ∇ ∇ ⋅ E − ∇ 2E = −∇ 2E r r 2 2 ∂ E ∇ E = µε 2 ∂t 2 plane wave equation with v = 1/ µε Plane EM Wave - Dr. Ray Kwok Traveling Wave x(f ± vt ) ≡ )u(f reverse / forward traveling wave ∂f ∂u = )u('f = )u('f ∂x ∂x ∂ 2f ∂u note: = )u("f = )u("f 1 2π 2π ∂x 2 ∂x x ± vt = x ± vt k λ λ ∂f ∂u = )u('f = ±vf )u(' 1 = ()kx ± 2πft ∂t ∂t k ∂ 2f ∂u 1 = ±vf )u(" = v2 )u("f = ± ()ωt ± kx ∂t 2 ∂t k 2 2 x(f ± vt ) = f ()ωt ± kx ∂ f 1 ∂ f r r = wave equation f ()ωt − k ⋅ r ∂x 2 v2 ∂t 2 (3D) Plane EM Wave - Dr. Ray Kwok Plane Wave r r 2 2 ∂ E ∇ E = µε Similarly for B or H field ∂t 2 r r r r r r (j ωt−k⋅ )r r 2 )t,r(E = Eoe 2 ∂ H r r ∇ H = µε 2 2 2 ∂t ∇ E = −k E r r r r r r H )t,r( = H e (j ωt−k⋅ )r ∂ 2E r o = −ω2E ∂t 2 − k 2 = −ω2µε k = ω µε ω 1 = v = k µε Plane EM Wave - Dr. Ray Kwok Source-free EM wave r r (j ωt−kz ) )t,r(E = xˆE e V/m in vacuum with no current source. o r What is H ? (j ωt−kz ) ∇× E = yˆ{− jkE oe } r r kE xˆ yˆ zˆ H )t,r( = yˆ o e (j ωt−kz ) r ∂ ∂ ∂ ωµ ∇ × E = k 1 1 µε ε 1 ∂x ∂y ∂z = = = = ≡ (j ωt−kz ) ωµ fλµ vµ µ µ η Eoe 0 0 r r r r ηηη = wave Eo (j ωt−kz ) ∇ × E = −jωµ H H )t,r( = yˆ e Impedance r η (j ωt −kz ) ∇ × E = yˆ{}− jkE oe r r µE B = µH = yˆ o e (j ωt−kz ) r r kE vµ H )t,r( = yˆ o e (j ωt−kz ) ωµ r r E )t,r(B = yˆ o e (j ωt−kz ) v Plane EM Wave - Dr. Ray Kwok EM wave properties r (1) E & H are in phase. r (j ωt−kz ) )t,r(E = xˆEoe r r E r r r H )t,r( = yˆ o e (j ωt−kz ) (2) E ⊥ H ⊥ k η kˆ = Eˆ × Hˆ r r E B )t,r( = yˆ o e (j ωt−kz ) v Index of refraction (3) E c c o = v = = Bo n εrµr E µ o = η = Ho ε Plane EM Wave - Dr. Ray Kwok Electromagnetic wave Plane EM Wave - Dr. Ray Kwok Earlier exercise r r H )t,r( = xˆ 01.0 cos( 900 t + β )z A/m in vacuum with no current source. What is f, λ, direction of propagation, E ? ω = 2 πf = 900, f = 143 Hz (1) E & H are in phase. λ = c/f = (3 x 10 8)/(143) = 2094 km r r r propagate to the –z direction (2) E ⊥ H ⊥ k r r kˆ = Eˆ × Hˆ ∇× H = jωε E E E(r) = a 3.77 cos[900t + 3(10 -6)z] V/m o = v y (3) Bo E o = η Ho ηo = 377 Ω Plane EM Wave - Dr. Ray Kwok Example r r H )t,r( = (xˆ 01.0 − ˆ 02.0y )sin( 10 9 t +βz − )1.0 A/m. What is E ? β = ω/c = 10 9/(3 x 10 8) = 3.33 rad/m r r r (1) E & H are in phase. 9 V/m )t,r(E = Eo sin(10 t + 33.3 z− )1.0 r r r y (2) E ⊥ H ⊥ k E ˆ ˆ ˆ 2xˆ + yˆ k = E× H x Eˆ = = .0 894 xˆ + .0 447 yˆ 5 H Eo (3) = v 2 2 2 → Ho = 0.01 + 0.02 Ho = 0.022 = Eo/ηo = E o/377 Bo Eo = 8.3 V/m E o = η r r 9 Ho )t,r(E = (3.8 xˆ .0 894 + yˆ .0 447 )sin( 10 t + 33.3 z − )1.0 η = 377 Ω r r o )t,r(E = (xˆ 4.7 + yˆ )7.3 sin( 10 9 t + 33.3 z − )1.0 V/m Plane EM Wave - Dr. Ray Kwok Exercise r r 8 )t,r(E = xˆ 20 cos( 10 t + z3 − )y V/m in non-magnetic material. What is H ? r r r (1) E & H are in phase. 8 H )t,r( = Ho cos( 10 t + z3 − )y A/m r r r y r (2) E ⊥ H ⊥ k k k = −3zˆ + yˆ ˆ ˆ ˆ E − 3yˆ − zˆ k = E× H z Hˆ = = − .0 949 yˆ − .0 316 zˆ 10 H v = ω/k = 10 8/√10 = 3.16 x 10 7 m/s Eo √ → 2 (3) = v v = c/n = c/ εr εr = (c/v) = 90 √ √ √ Bo η = (µ/ε ) = ηo/ εr = 377/ 90 = 39.7 E H = E /η = 20/39.7 =0.5 o = η o o Ho r r 8 η = 377 Ω H )t,r( = (5.0 −yˆ .0 949 − ˆ .0z 316 ) cos( 10 t + z3 − )y o r r H )t,r( = −(yˆ .0 475 + ˆ .0z 158 )cos( 10 8 t + z3 − )y A/m Plane EM Wave - Dr. Ray Kwok EM wave properties - generalized (1) E & H are in phase. r 1 r r r r H = kˆ × E (2) E ⊥ H ⊥ k η kˆ = Eˆ × Hˆ Index of refraction r r (3) E c c E = ηH × kˆ o = v = = Bo n εrµr E µ o = η = Ho ε Plane EM Wave - Dr. Ray Kwok Earlier exercise (free space) r r H )t,r( =0(xˆ . 01−0yˆ . 02)sin( 10 9 t + βz − )1.0 A/m. What is E ? β = ω/c = 10 9/(3 x 10 8) = 3.33 rad/m r r E = ηH× kˆ r E = 377 0(xˆ . 01−0yˆ . 02)sin( ωt + βz − )1.0 ×(−ˆ)z r 9 E =3(yˆ . 77+7xˆ . 54)sin( 10 3t + . 33z − )1.0 V/m. Plane EM Wave - Dr. Ray Kwok Earlier exercise r r 8 )t,r(E = xˆ 20 cos( 10 t + z3 − )y V/m in non-magnetic material. r What is H ? k = −3zˆ + yˆ v = ω/k = 10 8/√10 = 3.16 x 10 7 m/s √ → 2 v = c/n = c/ εr εr = (c/v) = 90 √ √ √ η = (µ/ε ) = ηo/ εr = 377/ 90 = 39.7 r 1 r H = kˆ × E η r 1 − 3zˆ + yˆ H = ×[]xˆ 20 cos ()10 8 t + z3 − y 39 7. 10 r H = ()− yˆ .0 478 − ˆ .0z 159 cos ()10 8 t + z3 − y A/m Plane EM Wave - Dr. Ray Kwok the work-energy theorem Poynting Theorem for electrodynamics Work done on a charge δδδq by EM force: r r r r r ∂H r r r ∂E E ⋅ J = −µH ⋅ − ∇ ⋅ ()E × H − εE ⋅ r r r r r r ∂t ∂t l r r dW = F ⋅ d = δq(E + v × B)⋅ dtv r r 2 2 r r r r µ ∂H ε ∂E E ⋅ J = − − − ∇ ⋅ ()E × H dW = δqE ⋅ vdt 2 ∂t 2 ∂t r r r r r r dW = ρδ V E ⋅ dtv = δVE ⋅ dtJ 2 2 r r () dW 1 ∂H ∂E = −∫ µ + ε dV − ∫∇ ⋅ ()E × H dV dW r r dt 2 ∂t ∂t = ∫ E ⋅ dVJ r r dt 2 2 r r r r dW 1 ∂H ∂E r r = −∫ µ + εo dV − ∫ ()E × H ⋅ ad ∂E dt 2 ∂t ∂t ∇ × H = Jf + ε ∂t r dW ∂U r r r r r r r ≡ − EM − S⋅ ad ∂E dt ∂t ∫ E ⋅ J = E ⋅∇ × H − εE ⋅ Poynting Vector ∂t r r r r r r (math) Power flow out of the enclosed surface ∇ ⋅ ()E × H = H ⋅∇ × E − E ⋅∇ × H EM power stored in the volume r r r r ∂H r r E ⋅ ∇ × H = H ⋅− µ − ∇ ⋅ ()E × H The decrease of the EM energy stored is to do work on ∂t a charge or due to the net energy escape through the surface. Plane EM Wave - Dr. Ray Kwok Poynting Vector r r r S ≡ E × H Magnitude gives power intensity = power/area Direction gives direction of propagation r 1 r r S ≡ ℜ E[e × H*] Time average ave 2 2 E η 2 S = o = H ave 2η 2 o This is similar to P = ½ (V 2/Z) = ½ ( I2Z) Plane EM Wave - Dr. Ray Kwok Example If solar illumination is characterized by a power density of 1 kW/m 2 at Earth’s surface, find (a) the total power radiated by the sun, (b) the total power intercepted by Earth, and (c) the electric field of the power density incident upon Earth’s surface, assuming that all the solar illumination is at a single frequency.
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]
  • Lecture 14: Polarization
    Matthew Schwartz Lecture 14: Polarization 1 Polarization vectors In the last lecture, we showed that Maxwell’s equations admit plane wave solutions ~ · − ~ · − E~ = E~ ei k x~ ωt , B~ = B~ ei k x~ ωt (1) 0 0 ~ ~ Here, E0 and B0 are called the polarization vectors for the electric and magnetic fields. These are complex 3 dimensional vectors. The wavevector ~k and angular frequency ω are real and in the vacuum are related by ω = c ~k . This relation implies that electromagnetic waves are disper- sionless with velocity c: the speed of light. In materials, like a prism, light can have dispersion. We will come to this later. In addition, we found that for plane waves 1 B~ = ~k × E~ (2) 0 ω 0 This equation implies that the magnetic field in a plane wave is completely determined by the electric field. In particular, it implies that their magnitudes are related by ~ ~ E0 = c B0 (3) and that ~ ~ ~ ~ ~ ~ k · E0 =0, k · B0 =0, E0 · B0 =0 (4) In other words, the polarization vector of the electric field, the polarization vector of the mag- netic field, and the direction ~k that the plane wave is propagating are all orthogonal. To see how much freedom there is left in the plane wave, it’s helpful to choose coordinates. We can always define the zˆ direction as where ~k points. When we put a hat on a vector, it means the unit vector pointing in that direction, that is zˆ=(0, 0, 1). Thus the electric field has the form iω z −t E~ E~ e c = 0 (5) ~ ~ which moves in the z direction at the speed of light.
    [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]
  • Physics 212 Lecture 24
    Physics 212 Lecture 24 Electricity & Magnetism Lecture 24, Slide 1 Your Comments Why do we want to polarize light? What is polarized light used for? I feel like after the polarization lecture the Professor laughs and goes tell his friends, "I ran out of things to teach today so I made some stuff up and the students totally bought it." I really wish you would explain the new right hand rule. I cant make it work in my mind I can't wait to see what demos are going to happen in class!!! This topic looks like so much fun!!!! With E related to B by E=cB where c=(u0e0)^-0.5, does the ratio between E and B change when light passes through some material m for which em =/= e0? I feel like if specific examples of homework were done for us it would help more, instead of vague general explanations, which of course help with understanding the theory behind the material. THIS IS SO COOL! Could you explain what polarization looks like? The lines that are drawn through the polarizers symbolize what? Are they supposed to be slits in which light is let through? Real talk? The Law of Malus is the most metal name for a scientific concept ever devised. Just say it in a deep, commanding voice, "DESPAIR AT THE LAW OF MALUS." Awesome! Electricity & Magnetism Lecture 24, Slide 2 Linearly Polarized Light So far we have considered plane waves that look like this: From now on just draw E and remember that B is still there: Electricity & Magnetism Lecture 24, Slide 3 Linear Polarization “I was a bit confused by the introduction of the "e-hat" vector (as in its purpose/usefulness)” Electricity & Magnetism Lecture 24, Slide 4 Polarizer The molecular structure of a polarizer causes the component of the E field perpendicular to the Transmission Axis to be absorbed.
    [Show full text]
  • 20 Polarization
    Utah State University DigitalCommons@USU Foundations of Wave Phenomena Open Textbooks 8-2014 20 Polarization Charles G. Torre Department of Physics, Utah State University, [email protected] Follow this and additional works at: https://digitalcommons.usu.edu/foundation_wave Part of the Physics Commons To read user comments about this document and to leave your own comment, go to https://digitalcommons.usu.edu/foundation_wave/3 Recommended Citation Torre, Charles G., "20 Polarization" (2014). Foundations of Wave Phenomena. 3. https://digitalcommons.usu.edu/foundation_wave/3 This Book is brought to you for free and open access by the Open Textbooks at DigitalCommons@USU. It has been accepted for inclusion in Foundations of Wave Phenomena by an authorized administrator of DigitalCommons@USU. For more information, please contact [email protected]. Foundations of Wave Phenomena, Version 8.2 of infinite radius. If we consider an isolated system, so that the electric and magnetic fields vanish sufficiently rapidly at large distances (i.e., “at infinity”), then the flux of the Poynting vector will vanish as the radius of A is taken to infinity. Thus the total electromagnetic energy of an isolated (and source-free) electromagnetic field is constant in time. 20. Polarization. Our final topic in this brief study of electromagnetic waves concerns the phenomenon of polarization, which occurs thanks to the vector nature of the waves. More precisely, the polarization of an electromagnetic plane wave concerns the direction of the electric (and magnetic) vector fields. Let us first give a rough, qualitative motivation for the phenomenon. An electromagnetic plane wave is a traveling sinusoidal disturbance in the electric and magnetic fields.
    [Show full text]
  • Basic Polarization Techniques and Devices
    Basic Polarization Techniques and Devices © 2005 Meadowlark Optics, Inc This application note briefly describes polarized light, retardation and a few of the tools used to manipulate the polarization state of light. Also included are descriptions of basic component combinations that provide common light manipulation tools such as optical isolators, light attenuators, polarization rotators and variable beam splitters. Light Polarization In classical physics, light of a single color is described by an electromagnetic field in which electric and magnetic fields oscillate at a frequency, (ν), that is related to the wavelength, (λ), as shown in the equation c = λν where c is the velocity of light. Visible light, for example, has wavelengths from 400-750 nm. An important property of optical waves is their polarization state. A vertically polarized wave is one for which the electric field lies only along the z-axis if the wave propagates along the y-axis (Figure 1A). Similarly, a horizontally polarized wave is one in which the electric field lies only along the x-axis. Any polarization state propagating along the y-axis can be superposed into vertically and horizontally polarized waves with a specific relative phase. The amplitude of the two components is determined by projections of the polarization direction along the vertical or horizontal axes. For instance, light polarized at 45° to the x-z plane is equal in amplitude and phase for both vertically and horizontally polarized light (Figure 1B). Page 1 of 7 Circularly polarized light is created when one linear electric field component is phase shifted in relation to the orthogonal component by λ/4, as shown in Figure 1C.
    [Show full text]
  • Elliptical Polarization
    Lecture 5: Polarization and Related Antenna Parameters (Polarization of EM fields – revision. Polarization vector. Antenna polarization. Polarization loss factor and polarization efficiency.) 1. Polarization of EM fields. The polarization of the EM field describes the time variations of the field vectors at a given point. In other words, it describes the way the direction and magnitude the field vectors (usually E ) change in time. The polarization is the figure traced by the extremity of the time- varying field vector at a given point. According to the shape of the trace, three types of polarization exist for harmonic fields: linear, circular and elliptical: y y y E E E ω z x z x z x (a) linear polarization (b) circular polarization (c) elliptical polarization Any type of polarization can be represented by two orthogonal linear polarizations, ( EExy, )or(EEHV, ), whose fields are out of phase by an angle δ of L . • δ = π IfL 0 or n , then a linear polarization results. • δπ= = If L /2 (90) and EExy, then a circular polarization results. • In the most general case, elliptical polarization is defined. 1 It is also true that any type of polarization can be represented by a right-hand circular and a left-hand circular polarizations (EELR , ). We shall revise the above statements and definitions, while introducing the new concept of polarization vector. 2. Field polarization in terms of two orthogonal linearly polarized components. The polarization of any field can be represented by a suitable set of two orthogonal linearly polarized fields. Assume that locally a far field propagates along the z-axis, and the field vectors have only transverse components.
    [Show full text]
  • Why Circular Polarization Antenna? FRC Polarization Types
    Why Circular Polarization Antenna? FRC Polarization Types An antenna is a transducer that converts radio frequency (RF) electric current to electromagnetic waves that are then radiated into space. Antenna polarization is an important consideration when selecting and installing antennas. Most wireless communication systems use either linear (vertical, horizontal) or circular polarization. Knowing the difference between polarizations can help maximize system performance for the user. Linear Polarization: An antenna is vertically linear polarized when its electric field is perpendicular to the Earth’s surface. An example of a vertical antenna is a broadcast tower for AM radio or the whip antenna on an automobile. Horizontally linear polarized antennas have their electric field parallel to the Earth's surface. For example, television transmissions in the USA use horizontal polarization. Thus, TV antennas are horizontally-oriented. Circular Polarization: In a circularly-polarized antenna, the plane of polarization rotates in a corkscrew pattern making one complete revolution during each wavelength. A circularly- polarized wave radiates energy in the horizontal, vertical planes as well as every plane in between. If the rotation is clockwise looking in the direction of propagation, the sense is called right-hand-circular (RHC). If the rotation is counterclockwise, the sense is called left-hand- circular (LHC). Advantages of Circular Polarization Reflectivity: Radio signals are reflected or absorbed depending on the material they come in contact with. Because linear polarized antennas are able to “attack" the problem in only one plane, if the reflecting surface does not reflect the signal precisely in the same plane, that signal strength will be lost.
    [Show full text]
  • UNIT 28: ELECTROMAGNETIC WAVES and POLARIZATION Approximate Time Three 100-Minute Sessions
    Name ______________________ Date(YY/MM/DD) ______/_________/_______ St.No. __ __ __ __ __-__ __ __ __ Section__________ Group #_____ UNIT 28: ELECTROMAGNETIC WAVES AND POLARIZATION Approximate Time Three 100-minute Sessions Hey diddle diddle, what kind of riddle Is this nature of light? Sometimes it’s a wave, Other times particle... But which answer will be marked right? Jon Scieszka OBJECTIVES 1. To understand electromagnetic waves and how they propagate. 2. To investigate different ways to polarize light including linear and circular polarization. © 2014 by S. Johnson. Adapted from PHYS 131 Optics Lab #3. Page 28-2 Studio Physics Activity Guide SFU OVERVIEW In this unit you will learn about the behaviour of electro- magnetic waves. Maxwell predicted the existence of elec- tromagnetic waves in 1864, a long time before anyone was able to create or detect them. It was Maxwell’s four famous equations that led him to this prediction which was finally confirmed experimentally by Hertz in 1887. Maxwell argued that if a changing magnetic field could create a changing electric field then the changing electric field would in turn create another changing magnetic field. He predicted that these changing fields would continuously generate each other and so propagate and carry energy with them. The mathematics involved further indicated that these fields would propagate as waves. When one solves for the wave speed one gets: 1 wave speed: c = ε0µ0 (28.1) Where ε0 and µ0 are the electrical constants we have already been introduced to. The magnitude of this speed led Max- well to€ further hypothesize that light is an electromagnetic wave.
    [Show full text]
  • Linear Or Circular Polarization? Michele Galletti, Dong Huang, and Pavlos Kollias
    628 IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING, VOL. 52, NO. 1, JANUARY 2014 Zenith/Nadir Pointing mm-Wave Radars: Linear or Circular Polarization? Michele Galletti, Dong Huang, and Pavlos Kollias Abstract—We consider zenith/nadir pointing atmospheric and receive the copolar and cross-polar components of the radars and explore the effects of different dual-polarization ar- backscattered signal. In the following, this polarimetric mode chitectures on the retrieved variables: reflectivity, depolarization (linear polarization transmission, co- and cross-pol receive) is ratio, cross-polar coherence, and degree of polarization. Under the assumption of azimuthal symmetry, when the linear depo- termed linear depolarization ratio (LDR) mode. The MMCR larization ratio (LDR) and circular depolarization ratio (CDR) operated at Ka band (35 GHz), transmitted circular polarization modes are compared, it is found that for most atmospheric scat- and received the copolar and cross-polar components of the terers reflectivity is comparable, whereas the depolarization ratio backscattered signal. Such operating mode is indicated with dynamic range is maximized at CDR mode by at least 3 dB. circular depolarization ratio (CDR) mode. In the presence of anisotropic (aligned) scatterers, that is, when azimuthal symmetry is broken, polarimetric variables at CDR Since most atmospheric scatterers tend to have a shape close mode do have the desirable property of rotational invariance to spherical, both LDR and CDR modes are characterized by a and, further, the dynamic range of CDR can be significantly large difference in signal power (generally larger than 20 dB) larger than the dynamic range of LDR. The physical meaning between the two receive polarimetric channels.
    [Show full text]
  • Polarization of Light Thursday, 11/09/2006 Physics 158 Peter Beyersdorf
    Polarization of Light Thursday, 11/09/2006 Physics 158 Peter Beyersdorf Document info 1 Class Outline Polarization of Light Polarization basis’ Jones Calculus 16. 2 Polarization The Electric field direction defines the polarization of light Since light is a transverse wave, the electric field can point in any direction transverse to the direction of propagation Any arbitrary polarization state can be considered as a superposition of two orthogonal polarization states (i.e. it can be described in different bases) 16. 3 Electric Field Direction Light is a transverse electromagnetic wave so the electric (and magnetic) field oscillates in a direction transverse to the direction of propagation Possible states of electric field polarization are Linear electric field Circular plane wave Elliptical Random 4 Examples of polarization states right hand circular horizontal (CW as seen from observer) left hand circular vertical (CCW as seen from observer) linear polarization at an elliptical arbitrary angle 16. 5 Linear Polarization Basis Any polarization state can be described as the sum of two orthogonal linear polarization states i(kz ωt+φx) Ex(z, t) = E0xˆie − i(kz ωt+φy ) Ey(z, t) = E0yˆje − ! iφxˆ iφy ˆ i(kz ωt) E(z, t) = Ex(z,!t) + Ey(z, t) = E0xe i + E0ye j e − " # ! !E0y=0 ! E0x=0 E0y=E0x E0y=-E0x y y y y x x x horizontal vertical diagonal diagonal φ φ φx=φy+π x= y 16. 6 Circular Polarization iφx iφy i(kz ωt) E(z, t) = E0xe ˆi + E0ye ˆj e − " # Fo!r the case |φx-φy|=π/2 the magnitude of the field doesn’t change, but the direction sweeps out a circle The polarization is said Left-Handed Right-Handed to be right-handed if y y it progresses clockwise as seen by an observer looking into the light.
    [Show full text]
  • Electromagnetic Waves & Polarization
    9/13/2017 Course Instructor Dr. Raymond C. Rumpf Office: A‐337 Phone: (915) 747‐6958 E‐Mail: [email protected] EE 4347 Applied Electromagnetics Topic 3a Electromagnetic Waves & Polarization Electromagnetic Waves & Polarization These notes may contain copyrighted material obtained under fair use rules. Distribution of these materials is strictly prohibited Slide 1 Lecture Outline • Maxwell’s Equations • Derivation of the Wave Equation • Solution to the Wave Equation • Intuitive Wave Parameters • Dispersion Relation • Electromagnetic Wave Polarization • Visualization of EM Waves Electromagnetic Waves & Polarization Slide 2 1 9/13/2017 Maxwell’s Equations Electromagnetic Waves & Polarization Slide 3 Recall Maxwell’s Equations in Source Free Media In source‐free media, we have and .J 0 v 0 Maxwell’s equations in the frequency‐domain become Curl Equations Divergence Equations Ej B D 0 Hj D B 0 Constitutive Relations DE BH Electromagnetic Waves & Polarization Slide 4 2 9/13/2017 The Curl Equations Predict Waves After substituting the constitutive relations into the curl equations, we get Ej H Hj E A time‐harmonic magnetic field will A time‐harmonic electric field will induce a time‐harmonic electric induce a time‐harmonic magnetic field circulating about the magnetic field circulating about the electric field. field. A time‐harmonic circulating electric A time‐harmonic circulating field will induce a time‐harmonic magnetic field will induce a time‐ magnetic field along the axis of harmonic electric field along the circulation. axis of circulation. An H induces an E. That E induces another H. That new H induces another E. That E induces yet another H.
    [Show full text]