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Electromagnetic Waves

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Presentation on theme: "Electromagnetic Waves"— Presentation transcript:

1 Electromagnetic Waves
Chapter 32 Electromagnetic Waves © 2016 Pearson Education Inc. – Modfied by Scott Hildreth – Chabot College 2017

2 Learning Goals for Chapter 32
How are electromagnetic waves generated? Why speed of light is related to fundamental E&M constants. Describe propagation of sinusoidal electromagnetic wave. Determine energy & momentum carried by EM wave. Describe standing electromagnetic waves. © 2016 Pearson Education Inc.

3 Introduction Why do metals reflect light? Visible light is EM wave.
Many other examples: x-rays, radiowaves, microwaves Unlike sound or waves on a string, EM waves do NOT require a medium to travel. © 2016 Pearson Education Inc.

4 James Clerk Maxwell Scottish physicist James Clerk Maxwell (1831–1879) shows fundamental nature of light mathematically Proved in 1865 EM “disturbance” propagates in free space w/ speed equal to “c” Deduced correctly that light was an electromagnetic wave © 2016 Pearson Education Inc.

5 Maxwell’s Equation’s in integral form
Gauss’s Law Gauss’s Law for Magnetism Faraday’s Law dS = n dA Flux = field integrated over a surface No magnetiic monopoles E .dl is an EMF (volts) Ampere’s Law

6 Maxwell’s Equations Differential Form

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8 Electricity, magnetism, and light
According to Maxwell’s equations, accelerating electric charge must produce electromagnetic waves. Overhead power lines carry strong AC; substantial amount of charge accelerates back & forth, generating EM (radio) waves. These waves can produce a buzzing sound from your car radio when you drive near the lines. © 2016 Pearson Education Inc.

9 Electromagnetic spectrum
Frequencies & wavelengths of EM waves in nature extend over wide range! Use logarithmic scale to show all bands. Boundaries between bands are (somewhat) arbitrary. © 2016 Pearson Education Inc.

10 Visible light Extends from violet end (400 nm) to red (700 nm).
© 2016 Pearson Education Inc.

11 Ultraviolet vision Many insects & birds can see UV that humans cannot.
Left photo shows how “black-eyed Susans” look to us. Right photo (in false color), taken with UV camera, shows how flowers appear to bees that pollinate them. Note prominent central spot invisible to humans. © 2016 Pearson Education Inc.

12 Ultraviolet vision

13 A simple plane electromagnetic wave
Imagine space divided into two regions by plane perpendicular to x-axis. At every point to left uniform electric & magnetic fields Boundary plane (wave front) moves in +x-direction with constant speed c. © 2016 Pearson Education Inc.

14 Gauss’s laws & simple plane wave
Create rectangular Gaussian surface simple plane wave is traveling through. Box encloses no electric charge. No flux! So E & B fields must be perpendicular to direction of propagation. Wave must be transverse. © 2016 Pearson Education Inc.

15 Faraday’s law & simple plane wave
In time dt, magnetic flux through rectangle in xy-plane increases by dΦB. Increase equals flux through shaded rectangle w/ area ac dt: dΦB = Bac dt So dΦB/dt = Bac Faraday’s law implies: © 2016 Pearson Education Inc.

16 Faraday’s Law

17 Ampere’s law & simple plane wave
In time dt, electric flux through rectangle in xz-plane increases by dΦE. Increase equals flux through shaded rectangle w/ area ac dt: dΦE = Eac dt Thus dΦE/dt = Eac and…. © 2016 Pearson Education Inc.

18 Properties of electromagnetic waves
Maxwell’s equations imply in an EM wave, BOTH E & B fields are perpendicular to direction of propagation of wave & to each other. For electromagnetic waves, ratio between magnitudes of electric & magnetic fields E = cB © 2016 Pearson Education Inc.

19 Properties of electromagnetic waves
Travel in vacuum with definite (and unchanging) speed: c = 3.00 × 108 m/s. Unlike mechanical waves, EM waves require no medium.

20 Properties of electromagnetic waves
Direction of propagation of EM wave is direction of vector cross product of electric & magnetic fields. © 2016 Pearson Education Inc.

21 Sinusoidal electromagnetic waves
EM waves produced by oscillating point charge are not plane waves. © 2016 Pearson Education Inc.

22 Sinusoidal electromagnetic waves
EM waves produced by oscillating point charge are not plane waves. Restrict observations to relatively small region of space at a sufficiently great distance from source, these waves are well approximated by plane waves. © 2016 Pearson Education Inc.

23 Fields of a sinusoidal wave
Linearly polarized, sinusoidal EM wave traveling +x-direction. One wavelength shown at time t = 0. Fields shown for a few points along x-axis. © 2016 Pearson Education Inc.

24 Polarization of sinusoidal wave
© 2016 Pearson Education Inc.

25 Variation in Polarization of sinusoidal wave
© 2016 Pearson Education Inc.

26 Elliptical Polarization of sinusoidal wave
© 2016 Pearson Education Inc.

27 Traveling sinusoidal EM waves
Describe EM waves with wave functions: Wave travels right w/ speed c = ω/k. Amplitudes related by: © 2016 Pearson Education Inc.

28 Electromagnetic waves in matter
When electromagnetic waves travel in nonconducting materials— dielectrics — speed v of waves depends on dielectric constant of material. Ratio of speed c in vacuum to speed v in material is index of refraction n © 2016 Pearson Education Inc.

29 Energy in electromagnetic waves
EM waves transport energy British physicist John Poynting introduced Poynting vector, S Magnitude of Poynting vector = power per unit area in wave [W/m2] Direction of Poynting vector = direction of propagation © 2016 Pearson Education Inc.

30 Energy in electromagnetic waves
British physicist John Poynting Worked with Maxwell Worked with JJ Thompson Wrote THE physics textbook used for 50+ years! Coined “greenhouse effect”! © 2016 Pearson Education Inc.

31 Energy in electromagnetic waves
Poynting vector, S Magnitude of Poynting vector = power per unit area [W/m2] [E] = Newtons/Coulomb (from F = qE!) [B] = Teslas = Newtons/[Coulomb-meter/sec] (from F = qvxB!!) [m0] = Tesla-meter/Amp (from Ampere’s Law !!!) [S] = (N/C) x (T) x (Amps/Tm) = N/m-sec = Nm/m2-sec = W/m2 © 2016 Pearson Education Inc.

32 Energy in electromagnetic waves
Magnitude of average value of = intensity [W/m2] Rooftop solar panels tilted face-on to sun so panels absorb maximum amount of wave energy. © 2016 Pearson Education Inc.

33 Electromagnetic radiation pressure
EM waves carry momentum & exert radiation pressure on a surface: © 2016 Pearson Education Inc.

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35 Electromagnetic radiation pressure
Solar Constant: 1370 W/m2 at Earth’s Surface If solar panels on earth-orbiting satellite are perpendicular to sunlight, & radiation completely absorbed, average radiation pressure is 4.7 × 10−6 N/m2 © 2016 Pearson Education Inc.

36 Electromagnetic radiation pressure

37 Solar Sails!

38 Standing waves in a cavity
Typical microwave oven @ 2.45 GHz sets up standing EM wave w/ λ = 12.2 cm Strongly absorbed by water! Because standing wave has nodes spaced λ/2 = 6.1 cm apart, food must be rotated while cooking. Otherwise, portion at a node — where E-field amplitude = 0 will remain cold! Measure the speed of light yourself using Butter – or Peeps! © 2016 Pearson Education Inc.

39 Standing electromagnetic waves
EM waves reflected by conductor or dielectric, leading to standing waves. Remember E field in conductor MUST be zero!! So E(ends) = 0 permanently! Just like displacement wavefunction for closed pipes! © 2016 Pearson Education Inc.

40 Standing electromagnetic waves
Pattern does not move; instead, at every point E & B field vectors oscillate. © 2016 Pearson Education Inc.


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