What is a wave? f(x) f(x-3) f(x-2) f(x-1) x

Slides:



Advertisements
Similar presentations
Electromagnetic Waves in Conducting medium
Advertisements

NASSP Self-study Review 0f Electrodynamics
Chapter 1 Electromagnetic Fields
Lecture 8: Reflection and Transmission of Waves
PH0101 UNIT 2 LECTURE 31 PH0101 Unit 2 Lecture 3  Maxwell’s equations in free space  Plane electromagnetic wave equation  Characteristic impedance 
EEE 498/598 Overview of Electrical Engineering
Electromagnetic Waves
Chapter 4: Wave equations
The Propagation of Light
Electromagnetic Waves Physics 4 Prepared by Vince Zaccone For Campus Learning Assistance Services at UCSB.
Chapter 16 Wave Motion.
Physics 1402: Lecture 26 Today’s Agenda Announcements: Midterm 2: NOT Nov. 6 –About Monday Nov. 16 … Homework 07: due Friday this weekHomework 07: due.
6. Standing Waves, Beats, and Group Velocity Group velocity: the speed of information Going faster than light... Superposition again Standing waves: the.
1 Sinusoidal Waves The waves produced in SHM are sinusoidal, i.e., they can be described by a sine or cosine function with appropriate amplitude, frequency,
Waves, the Wave Equation, and Phase Velocity What is a wave? Forward [ f(x-vt) ] and backward [ f(x+vt) ] propagating waves The one-dimensional wave equation.
Feb. 2, 2011 Rosseland Mean Absorption Poynting Vector Plane EM Waves The Radiation Spectrum: Fourier Transforms.
Waves can be represented by simple harmonic motion.
LESSON 4 METO 621. The extinction law Consider a small element of an absorbing medium, ds, within the total medium s.
Feb. 7, 2011 Plane EM Waves The Radiation Spectrum: Fourier Transforms.
08/28/2013PHY Lecture 011 Light is electromagnetic radiation! = Electric Field = Magnetic Field Assume linear, isotropic, homogeneous media.
Electromagnetic Waves Electromagnetic waves are identical to mechanical waves with the exception that they do not require a medium for transmission.
Scalar and Vector Fields
1 Optical Properties of Materials … reflection … refraction (Snell’s law) … index of refraction Index of refraction Absorption.
EE3321 ELECTROMAGNETIC FIELD THEORY
The Electromagnetic Field. Maxwell Equations Constitutive Equations.
Prof. David R. Jackson Dept. of ECE Fall 2013 Notes 17 ECE 6340 Intermediate EM Waves 1.
Electromagnetic waves Physics 2102 Gabriela González.
Modern Optics I – wave properties of light
Chapter 34 Electromagnetic Waves. Currents produce B Change in E produces B Currents produce B Change in E produces B Change in B produces an E charges.
Time variation Combining electrostatics and magnetostatics: (1) .E =  /  o where  =  f +  b (2) .B = 0“no magnetic monopoles” (3)  x E = 0 “conservative”
The Hong Kong Polytechnic University Optics II----by Dr.H.Huang, Department of Applied Physics1 Light Waves Nature of Light: Light can be viewed as both.
Superposition of Sinusoidal Waves Let us now apply the principle of superposition to two sinusoidal waves travelling in the same direction in a linear.
2. Waves, the Wave Equation, and Phase Velocity What is a wave? Forward [ f(x-vt) ] and backward [ f(x+vt) ] propagating waves The one-dimensional wave.
Mussel’s contraction biophysics. Kinematics and dynamics rotation motion. Oscillation and wave. Mechanical wave. Acoustics.
1 ECE 480 Wireless Systems Lecture 3 Propagation and Modulation of RF Waves.
Oscillations & Waves IB Physics. Simple Harmonic Motion Oscillation 4. Physics. a. an effect expressible as a quantity that repeatedly and regularly.
1 Chapter 2 Wave motion August 25,27 Harmonic waves 2.1 One-dimensional waves Wave: A disturbance of the medium, which propagates through the space, transporting.
1 Chapter 3 Electromagnetic Theory, Photons and Light September 5,8 Electromagnetic waves 3.1 Basic laws of electromagnetic theory Lights are electromagnetic.
Waves, the Wave Equation, and Phase Velocity What is a wave? Forward [ f(x-vt) ] and backward [ f(x+vt) ] propagating waves The one-dimensional wave equation.
Electromagnetic Waves and Their Propagation Through the Atmosphere
Enhancing One‐Dimensional FDTD
So far, we have considered plane waves in an infinite homogeneous medium. A natural question would arise: what happens if a plane wave hits some object?
Chapter 16 Lecture One: Wave-I HW1 (problems): 16.12, 16.24, 16.27, 16.33, 16.52, 16.59, 17.6, Due.
Maxwell's Equations & Light Waves
Lecture 42: FRI 04 DEC Final Exam Review II Physics 2113 Jonathan Dowling.
Introduction to materials physics #3
Wave Dispersion EM radiation Maxwell’s Equations 1.
PHYS 408 Applied Optics (Lecture 3) JAN-APRIL 2016 EDITION JEFF YOUNG AMPEL RM 113.
Chapter 4: Wave equations
Electromagnetism Around 1800 classical physics knew: - 1/r 2 Force law of attraction between positive & negative charges. - v ×B Force law for a moving.
Preliminary mathematics: PHYS 344 Homework #1 Due in class Wednesday, Sept 9 th Read Chapters 1 and 2 of Krane, Modern Physics Problems: Chapter 2: 3,
1 EEE 431 Computational Methods in Electrodynamics Lecture 13 By Dr. Rasime Uyguroglu
Review of Waves Waves are of three main types: 1. Mechanical waves. We encounter these almost constantly. Examples: sound waves, water waves, and seismic.
7. Electromagnetic Waves 7A. Plane Waves Consider Maxwell’s Equations with no sources We are going to search for waves of the form To make things as general.
EE231 Introduction to Optics: Basic EM Andrea Fratalocchi ( slide 1 EE 231 Introduction to Optics Review of basic EM concepts Andrea.
2. Maxwell's Equations and Light Waves
Chapter 1 Electromagnetic Fields
Plane electromagnetic waves
Review of basic EM concepts
Notes 17 ECE 6340 Intermediate EM Waves Fall 2016
PLANE WAVE PROPAGATION
Lecture 14 : Electromagnetic Waves
Waves, the Wave Equation, and Phase Velocity
Lect. 06 phase & group velocities
Electromagnetic waves
Review of basic EM concepts
Lect.03 Time Varying Fields and Maxwell’s Equations
Optics 430/530, week II Plane wave solution of Maxwell’s equations
1st Week Seminar Sunryul Kim Antennas & RF Devices Lab.
Presentation transcript:

What is a wave? f(x) f(x-3) f(x-2) f(x-1) x A wave is anything that moves. To displace any function f(x) to the right, just change its argument from x to x-a, where a is a positive number. If we let a = v t, where v is positive and t is time, then the displacement will increase with time. So represents a rightward, or forward, propagating wave. Similarly, represents a leftward, or backward, propagating wave, where v is the velocity of the wave. f(x) f(x-3) f(x-2) f(x-1) x 0 1 2 3 f(x - v t) Picture courtesy of the Consortium for Optics and Imaging Education f(x + v t) For an EM wave, we could have E = f(x ± vt)

The one-dimensional wave equation The one-dimensional wave equation for scalar (i.e., non-vector) functions, f: where v will be the velocity of the wave. The wave equation has the simple solution: where f (u) can be any twice-differentiable function.

Proof that f (x ± vt) solves the wave equation Write f (x ± vt) as f (u), where u = x ± vt. So and   Now, use the chain rule: So Þ and Þ    Substituting into the wave equation:

What about a harmonic wave? E0 = wave amplitude (related to the energy carried by the wave). = angular wavenumber (λ = wavelength; = wavenumber = 1/λ) Alternatively: Where ω = kc = 2πc/λ = 2πf = angular frequency (f = frequency)

What about a harmonic wave? The argument of the cosine function represents the phase of the wave, ϕ, or the fraction of a complete cycle of the wave. In-phase waves Line of equal phase = wavefront = contours of maximum field Out-of-phase waves

The Phase Velocity v = l f v = w / k How fast is the wave traveling? Velocity is a reference distance divided by a reference time. The phase velocity is the wavelength / period: v = l / t Since f = 1/t : In terms of k, k = 2p / l, and the angular frequency, w = 2p / t, this is: v = l f v = w / k

The Group Velocity This is the velocity at which the overall shape of the wave’s amplitudes, or the wave ‘envelope’, propagates. (= signal velocity) Here, phase velocity = group velocity (the medium is non-dispersive)

Dispersion: phase/group velocity depends on frequency Black dot moves at phase velocity. Red dot moves at group velocity. This is normal dispersion (refractive index decreases with increasing λ)

Dispersion: phase/group velocity depends on frequency Black dot moves at group velocity. Red dot moves at phase velocity. This is anomalous dispersion (refractive index increases with increasing λ)

Normal dispersion of visible light Shorter (blue) wavelengths refracted more than long (red) wavelengths. Refractive index of blue light > red light.

Complex numbers Let the x-coordinate be the real part Consider a point, P = (x,y), on a 2D Cartesian grid. Let the x-coordinate be the real part and the y-coordinate the imaginary part of a complex number. So, instead of using an ordered pair, (x,y), we write: P = x + i y = A cos(j) + i A sin(j) where i = √(-1) …or sometimes j = √(-1)

exp(ij) = cos(j) + i sin(j) Euler’s Formula Voted the ‘Most Beautiful Mathematical Formula Ever’ in 1988 Links the trigonometric functions and the complex exponential function exp(ij) = cos(j) + i sin(j) so the point, P = A cos(j) + i A sin(j), can also be written: P = A exp(ij) = A eiφ where A = Amplitude j = Phase

Waves using complex numbers The argument of the cosine function represents the phase of the wave, ϕ, or the fraction of a complete cycle of the wave. Using complex numbers, we can write the harmonic wave equation as: i.e., E = E0 cos(j) + i E0 sin(j), where the ‘real’ part of the expression actually represents the wave. We also need to specify the displacement E at x = 0 and t = 0, i.e., the ‘initial’ displacement.

Amplitude and Absolute phase E(x,t) = A cos[(k x – w t ) – q ] A = Amplitude q = Absolute phase (or initial, constant phase) at x = 0, t =0 p kx

Definitions Spatial quantities: Temporal quantities:

Complex number theorems

More complex number theorems Any complex number, z, can be written: z = Re{ z } + i Im{ z } So Re{ z } = 1/2 ( z + z* ) and Im{ z } = 1/2i ( z – z* ) where z* is the complex conjugate of z ( i ® –i ) The "magnitude," | z |, of a complex number is: | z |2 = z z* = Re{ z }2 + Im{ z }2 To convert z into polar form, A exp(ij): A2 = Re{ z }2 + Im{ z }2 tan(j) = Im{ z } / Re{ z }

Waves using complex numbers So the electric field of an EM wave can be written: E(x,t) = E0 cos(kx – wt – q) Since exp(ij) = cos(j) + i sin(j), E(x,t) can also be written: E(x,t) = Re { E0 exp[i(kx – wt – q)] } Recall that the energy transferred by a wave (flux density) is proportional to the square of the amplitude, i.e., E02. Only the interaction of the wave with matter can alter the energy of the propagating wave. Remote sensing exploits this modulation of energy.

Waves using complex amplitudes We can let the amplitude be complex: Where the constant stuff is separated from the rapidly changing stuff. The resulting "complex amplitude”: is constant in this case (as E0 and θ are constant), which implies that the medium in which the wave is propagating is nonabsorbing. What happens to the wave amplitude upon interaction with matter?

Complex numbers simplify waves! Adding waves of the same frequency, but different initial phase, yields a wave of the same frequency. This isn't so obvious using trigonometric functions, but it's easy with complex exponentials: where all initial phases are lumped into E1, E2, and E3.

Vector fields However, light is a 3D vector field. A 3D vector field assigns a 3D vector (i.e., an arrow having both direction and length) to each point in 3D space. A light wave has both electric and magnetic 3D vector fields: And it can propagate in any direction, and point in any direction in space.

The 3D wave equation for the electric field and its solution A light wave can propagate in any direction in space. So we must allow the space derivative to be 3D: whose solution is:   Where is a constant, complex vector And is a complex wave vector – the length of this vector is inversely proportional to the wavelength of the wave. Its magnitude is the angular wavenumber, k = 2π/λ. is a position vector

The 3D wave equation for the electric field and its solution The vector is normal to planes of constant phase (and hence indicates the direction of propagation of wave crests) The vector is normal to planes of constant amplitude. Note that these are not necessarily parallel. The amplitude of the wave at location is now: So if is zero, then the medium is nonabsorbing, since the amplitude is constant .

EM propagation in homogeneous materials The speed of an EM wave in free space is given by: 0 = permittivity of free space, 0 = magnetic permeability of free space To describe EM propagation in other media, two properties of the medium are important, its electric permittivity ε and magnetic permeability μ. These are also complex parameters.  = 0(1+ ) + i = complex permittivity = electric conductivity = electric susceptibility (to polarization under the influence of an external field) Note that ε and μ also depend on frequency (ω).

Vector Waves We must now allow the field E and its complex field amplitude to be vectors: The complex vector amplitude has six numbers that must be specified to completely determine it! x-component y-component z-component

The 1D wave equation for light waves where E is the light electric field We’ll use cosine- and sine-wave solutions:   or where: The speed of light in vacuum, usually called “c”, is 3 x 1010 cm/s.

Human wave Picture courtesy of the Consortium for Optics and Imaging Education A typical human wave has a phase velocity of about 20 seats per second.

The Phase of a Wave The phase is everything inside the cosine. E(x,t) = A cos(j), where j = k x – w t – q j = j(x,y,z,t) and is not a constant, like q ! In terms of the phase, w = – ¶j /¶t k = ¶j /¶x And – ¶j /¶t v = ––––––– ¶j /¶x This formula is useful when the wave is really complicated.

Usually, we just draw lines; it’s easier. is called a plane wave. A plane wave’s contours of maximum field, called wave-fronts or phase-fronts, are planes. They extend over all space. Wave-fronts are helpful for drawing pictures of interfering waves. A wave's wave-fronts sweep along at the speed of light. Usually, we just draw lines; it’s easier. A plane wave's wave-fronts are equally spaced, a wavelength apart. They're perpendicular to the propagation direction.

EM propagation in homogeneous materials In a non-vacuum, the wave must still satisfy Maxwell’s Equations: We can now define the complex index of refraction, N, as the ratio of the wave velocity in free space to the velocity in the medium: If the imaginary part of N is zero, the material is nonabsorbing, and v is the phase velocity of the wave in the medium. For most physical media, N > 1 (i.e., the speed of light is reduced relative to a vacuum). NB. N is a property of a particular medium and also a function of ω

EM propagation in homogeneous materials Relationships between the wave vector and the refractive index (these are derived from Maxwell’s Equations): These are the so-called ‘dispersion relations’ relating wavelength, frequency, velocity and refractive index. Real part of wave vector Imaginary part of wave vector

Absorption of EM radiation Recall the expression for the flux density of an EM wave (Poynting vector): When absorption occurs, the flux density of the absorbed frequencies is reduced.

Absorption of EM radiation The scalar amplitude of an EM wave at location is: From the expression for the flux density we have:

Absorption of EM radiation Now substitute the expression for : And we have: For a plane wave propagating in the x-direction.

Absorption coefficient and skin depth Where βa is known as the absorption coefficient: The quantity 1/βa gives the distance required for the wave’s energy to be attenuated to e-1 or ~37% of its original value, or the absorption/skin depth. It’s a function of frequency/wavelength.

Absorption coefficient and skin depth Within a certain material, and EM wave with λ = 1 µm is attenuated to 10% of its original intensity after propagating 1 cm. Determine the imaginary part of the refractive index ni. Solution is that ni = 1.8x10-5

Refractive index (n) – the dispersion equation qe = charge on an electron ε0 = electric constant m = mass of an electron Nk = number of charges (oscillators) of type k per unit volume ω = angular frequency of the EM radiation ωk = resonant frequency of an electron bound in an atom γ = ‘damping coefficient’ for oscillator k (oscillation cannot be permanent) What is the refractive index of visible light in air? What happens as the frequency of EM radiation increases at constant ωk? What happens if the resonant frequency is in the visible range? What happens if  > k? e.g., shine x-rays on glass, or radio waves on free electrons.

Refractive index (n) of water and ice

Penetration depth of water and ice (also called absorption depth or skin depth)