electromagnetic spectrum basics
DESCRIPTION
Electromagnetic Spectrum Basics. H. Paul Shuch Visiting Professor of Physics and Astronomy Lycoming College. Lesson Objectives Upon completion of this lesson, you will demonstrate mastery by: Deriving and recalling the speed of light - PowerPoint PPT PresentationTRANSCRIPT
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
ElectromagneticSpectrum Basics
H. Paul ShuchH. Paul Shuch
Visiting Professor of Physics and AstronomyVisiting Professor of Physics and Astronomy
Lycoming CollegeLycoming College
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
Lesson Objectives
Upon completion of this lesson, you will Upon completion of this lesson, you will demonstrate mastery by: demonstrate mastery by: • Deriving and recalling the speed of light Deriving and recalling the speed of light • Identifying the frequencies and wavelengths Identifying the frequencies and wavelengths defining the RF, Microwave, and visible spectra defining the RF, Microwave, and visible spectra • Converting between frequency and wavelengthConverting between frequency and wavelength• Knowing Planck's Constant from memory Knowing Planck's Constant from memory • Calculating the energy and mass of a photonCalculating the energy and mass of a photon
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
All waves behaveFundamentallyAlike GaussGauss
FaradayFaraday
AmpereAmpere
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
A continuum -- DC to Daylight . . .
and Beyond!
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
Visible Light
Less than one octave
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
= Frequency:Cycles per Second (Hz)
= Wavelength:Meters per Cycle
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
c =
Speed of Light
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
c = (both equal 3 * 108 m/s!)
Red: 750 nm * 400 THzViolet: 400 nm * 750 THz
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
(or three hundred kilometers per millisecond)
(that’s three hundred million meters per second)
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
The long and the short of it
The Rest of the Spectrum
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
The RF Spectrum
LLFF
EEHH
FF
MM
FF
HH
FF
VVHH
FF
UUHH
FF
SSHH
FF
VVLLFF
UULLFF
SSLLFF
EELLFF
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
RF Frequencies
LLFF
EEHH
FF
MM
FF
HH
FF
VVHH
FF
UUHH
FF
SSHH
FF
VVLLFF
UULLFF
SSLLFF
EELLFF
3 30 300 3 30 300 3 30 300 3 30 3003 30 300 3 30 300 3 30 300 3 30 300
Hz Hz Hz kHz kHz kHz MHz MHz MHz GHz GHz GHzHz Hz Hz kHz kHz kHz MHz MHz MHz GHz GHz GHz
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
RF Wavelengths
LLFF
EEHH
FF
MM
FF
HH
FF
VVHH
FF
UUHH
FF
SSHH
FF
VVLLFF
UULLFF
SSLLFF
EELLFF
100 10 1 100 10 1 100 10 1 10 1 1100 10 1 100 10 1 100 10 1 10 1 1
Mm Mm Mm km km km m m m cm cm mmMm Mm Mm km km km m m m cm cm mm m) = m) = 300 / 300 / (MHz)(MHz)
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
KuKu mmmmLL SS CC XX
1 GHz 100 GHz1 GHz 100 GHzLumped Lumped
ComponentsComponents
Distributed Distributed
ComponentsComponents
Optical Optical
ComponentsComponents
Microwave Bands
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
KuKu mmmmLL SS CC XX
GHz: 1 2 4 8 12 18 100GHz: 1 2 4 8 12 18 100
Microwave Bands
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
KuKu mmmmLL SS CC XX
cm: 30 15 7.5 3.75 2.5 1.67 0.3cm: 30 15 7.5 3.75 2.5 1.67 0.3
cm) cm) = 30 / = 30 / (GHz)(GHz)
GHz: 1 2 4 8 12 18 100GHz: 1 2 4 8 12 18 100
Microwave Bands
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
Microwave Band’sGreatest Hits
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
Actually, both!
Photons: are they waves, or particles?
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
Where h = 6.626 * 10-34 Joules * seconds
Energy per Photon –Planck’s Law
e = h
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
Remember red light?energy per photon
e = h * νe = (6.626 * 10-34 J * s) * (400 * 1012 cycles/s)e = 2.65 * 10-19 Joules
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
How about violet?energy per photon
e = h * νe = (6.626 * 10-34 J * s) * (750 * 1012 cycles/s)e = 4.97 * 10-19 Joules
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
How much energyper visible photon?
Less than a billionth of a billionth of a Joule!
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
Sunlight falling on Earth: ~ 1 kW/m2
(billions and billions of photons per secondper square meter!)
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
Left to right,Low to high energies
The spectrum asAn energy continuum
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
Q: How are Photonslike quick Catholics?
A: They have relativistic mass!A: They have relativistic mass!
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
(OK, so the rest mass of a photon is zero. However…)
e = h and e = m c2
so, h = m c2
and relativistic mass: m = h/c2
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
Let’s calculate relativistic mass for a red photon:
m = h/c2
= (6.626 * 10-34 J * s) * (400 * 1012 Hz) (3 * 108 m/s)2
= 2.94 * 10-36 kg
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
Is a red photon massive?
(no, that’s only about a millionth of the mass of an electron!)
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
Review Review ExercisesExercises
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
1. What is the velocity of forward propagation of radiant electromagnetic energy in free space?
c = 3 * 10c = 3 * 1088 m/s m/s
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
2. From memory, what frequencies and wave-lengths define the edges of the visible light spectrum? = 400 - 750 THz= 400 - 750 THz
= 750 - 400 nm= 750 - 400 nm
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
3. What is the value of Planck's Constant?
h = 6.626 * 10h = 6.626 * 10-34-34 J*s J*s
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
4. Interstellar hydrogen emits a strong spectral radiation line at a wavelength of 21 cm. To what frequency does this correspond? = c / = c /
= 1420 MHz= 1420 MHz
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
5. Interstellar hydrogen emits a strong spectral radiation line in which segment of the electromagnetic spectrum?1420 MHz is in the UHF spectrum, 1420 MHz is in the UHF spectrum, which extends from 300 to 3000 MHz.which extends from 300 to 3000 MHz.
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
6. Interstellar hydrogen emits a strong spectral radiation line in which microwave band?
21 cm is in L-band, which extends 21 cm is in L-band, which extends from 30 to 15 cm wavelength.from 30 to 15 cm wavelength.
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
7. Hydrogen line receiving equipment would be composed of which type of components?
All microwave circuitry incorporates All microwave circuitry incorporates distributed components.distributed components.
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
8. How much energy is emitted by one hydrogen photon? e = h * ν
e = (6.626 * 10-34 J*s) * (1.420 * 109 Hz)e = 9.4 * 10e = 9.4 * 10-25-25 Joules Joules
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
9. How much does that hydrogen photon weigh?
m = h/c2
= (6.626 * 10-34 J * s) * (1.42 * 109 Hz) (3 * 108 m/s)2
= 1.05 * 10-41 kg
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
10. What is the most important characteristic of all electromagnetic waves?
They all behave fundamentally alike.
Copyright © 2007 by H. Paul Shuch, Ph.D. All Rights Reserved
Did you score eight or higher?
You’ve mastered You’ve mastered spectrum basics!spectrum basics!