Transcript Slide 1

Electromagnetic Waves
Physics 6C
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Electromagnetic Waves
Electromagnetic (EM) waves are produced by an alternating current in a
wire. As the charges in the wire oscillate back and forth, the electric
field around them oscillates as well, in turn producing an oscillating
magnetic field. This magnetic field is always perpendicular to the
electric field, and the EM wave propagates perpendicular to both the Eand B-fields. This gives us a right-hand-rule relating the directions of
these 3 vectors:
1) Point the fingers of your right hand in the direction of the E-field
2) Curl them toward the B-field.
3) Stick out your thumb - it points in the direction of propagation.
Click here for an EM wave animation
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Like any other wave, we know the relationship
between the wavelength and frequency, and
the speed of propagation of the wave:
vwave  f  
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Like any other wave, we know the relationship
between the wavelength and frequency, and
the speed of propagation of the wave:
vwave  f  
In the case of EM waves, it turns out that
the wave speed is the speed of light.
So our formula for EM waves (in vacuum) is:
c  f  ; c 
1
 3  108 m
s
0  0
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Like any other wave, we know the relationship
between the wavelength and frequency, and
the speed of propagation of the wave:
vwave  f  
In the case of EM waves, it turns out that
the wave speed is the speed of light.
So our formula for EM waves (in vacuum) is:
c  f  ; c 
1
 3  108 m
s
0  0
It turns out that the speed of light is
also the ratio of the strengths of the
Electric and Magnetic fields in an EM
wave. So we know that E=cB (in
standard metric units)
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Like any other wave, we know the relationship
between the wavelength and frequency, and
the speed of propagation of the wave:
vwave  f  
In the case of EM waves, it turns out that
the wave speed is the speed of light.
So our formula for EM waves (in vacuum) is:
c  f  ; c 
1
 3  108 m
s
0  0
It turns out that the speed of light is
also the ratio of the strengths of the
Electric and Magnetic fields in an EM
wave. So we know that E=cB (in
standard metric units)
The continuum of various
wavelengths and frequencies for
EM waves is called the
Electromagnetic Spectrum
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Examples:
• Find the frequency of blue light with a wavelength of 460 nm.
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Examples:
• Find the frequency of blue light with a wavelength of 460 nm.
3  108 m
c
s
c  f   f  
 6.5  1014Hz
 460  109m
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Examples:
• Find the frequency of blue light with a wavelength of 460 nm.
3  108 m
c
s
c  f   f  
 6.5  1014Hz
 460  109m
• A cell phone transmits at a frequency of 1.25x108 Hz.
What is the wavelength of this EM wave?
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Examples:
• Find the frequency of blue light with a wavelength of 460 nm.
3  108 m
c
s
c  f   f  
 6.5  1014Hz
 460  109m
• A cell phone transmits at a frequency of 1.25x108 Hz.
What is the wavelength of this EM wave?
8m
3  10
c
s
c  f     
 2.4m
8
f 1.25  10 Hz
You will need to use this formula very often to convert
back and forth between frequency and wavelength.
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Energy and momentum in EM Waves
Electromagnetic waves transport energy. The energy associated with a wave is stored in
the oscillating electric and magnetic fields.
We will find out later that the frequency of the wave determines the amount of energy
that it carries. Since the EM wave is in 3-D, we need to measure the energy density
(energy per unit volume).
u
2
1

E
2 0
 21 B2  0E2 
0
1
0
B2
Note that the energy can be written in a few equivalent forms. Each can be useful,
depending on the information you know about the wave.
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Energy and momentum in EM Waves
Electromagnetic waves transport energy. The energy associated with a wave is stored in
the oscillating electric and magnetic fields.
We will find out later that the frequency of the wave determines the amount of energy
that it carries. Since the EM wave is in 3-D, we need to measure the energy density
(energy per unit volume).
u
2
1

E
2 0
 21 B2  0E2 
0
1
0
B2
This is the energy per unit volume
Note that the energy can be written in a few equivalent forms. Each can be useful,
depending on the information you know about the wave.
We can also talk about the intensity of an EM wave (for light we would think of it as
brightness). Just as for sound, intensity is measured as average power/area.
I
Power
 uc
Area
Just multiply the energy equation above
by the speed of light to get the intensity.
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Example: High-Energy Cancer Treatment
Scientists are working on a technique to kill cancer cells by zapping them with ultrahighenergy pulses of light that last for an extremely short amount of time. These short pulses
scramble the interior of a cell without causing it to explode, as long pulses do.
We can model a typical such cell as a disk 5.0 µm in diameter, with the pulse lasting for
4.0 ns with an average power of 2.0x1012 W. We shall assume that the energy is spread
uniformly over the faces of 100 cells for each pulse.
a) How much energy is given to the cell during this pulse?
b) What is the intensity (in W/m2) delivered to the cell?
c) What are the maximum values of the electric and magnetic fields in the pulse?
Prepared by Vince Zaccone
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Example: High-Energy Cancer Treatment
Scientists are working on a technique to kill cancer cells by zapping them with ultrahighenergy pulses of light that last for an extremely short amount of time. These short pulses
scramble the interior of a cell without causing it to explode, as long pulses do.
We can model a typical such cell as a disk 5.0 µm in diameter, with the pulse lasting for
4.0 ns with an average power of 2.0x1012 W. We shall assume that the energy is spread
uniformly over the faces of 100 cells for each pulse.
a) How much energy is given to the cell during this pulse?
b) What is the intensity (in W/m2) delivered to the cell?
c) What are the maximum values of the electric and magnetic fields in the pulse?
Recall that power is energy/time. So 2.0x1012 W is 2.0x1012 Joules/sec.
Energy  (2.0  101 2 sJ )  (4.0  109 s)  8  103 J  8000J
This is the total energy, which is spread out over 100 cells, so the
energy for each individual cell is 80 Joules.
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Example: High-Energy Cancer Treatment
Scientists are working on a technique to kill cancer cells by zapping them with ultrahighenergy pulses of light that last for an extremely short amount of time. These short pulses
scramble the interior of a cell without causing it to explode, as long pulses do.
We can model a typical such cell as a disk 5.0 µm in diameter, with the pulse lasting for
4.0 ns with an average power of 2.0x1012 W. We shall assume that the energy is spread
uniformly over the faces of 100 cells for each pulse.
a) How much energy is given to the cell during this pulse?
b) What is the intensity (in W/m2) delivered to the cell?
c) What are the maximum values of the electric and magnetic fields in the pulse?
To get intensity, we need to divide power/area. The area for a cell is
just the area of a circle:
Area  r2    (2.5  106 m)2  2.0  101 1m2
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Example: High-Energy Cancer Treatment
Scientists are working on a technique to kill cancer cells by zapping them with ultrahighenergy pulses of light that last for an extremely short amount of time. These short pulses
scramble the interior of a cell without causing it to explode, as long pulses do.
We can model a typical such cell as a disk 5.0 µm in diameter, with the pulse lasting for
4.0 ns with an average power of 2.0x1012 W. We shall assume that the energy is spread
uniformly over the faces of 100 cells for each pulse.
a) How much energy is given to the cell during this pulse?
b) What is the intensity (in W/m2) delivered to the cell?
c) What are the maximum values of the electric and magnetic fields in the pulse?
To get intensity, we need to divide power/area. The area for a cell is
just the area of a circle:
Area  r2    (2.5  106 m)2  2.0  101 1m2
Now divide to get intensity:
Power
2.0  101 2W
21 W
Intensity 


1
.
0

10
m2
100  r2 2.0  109 m2
This is the total area
of all 100 cells.
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Example: High-Energy Cancer Treatment
Scientists are working on a technique to kill cancer cells by zapping them with ultrahighenergy pulses of light that last for an extremely short amount of time. These short pulses
scramble the interior of a cell without causing it to explode, as long pulses do.
We can model a typical such cell as a disk 5.0 µm in diameter, with the pulse lasting for
4.0 ns with an average power of 2.0x1012 W. We shall assume that the energy is spread
uniformly over the faces of 100 cells for each pulse.
a) How much energy is given to the cell during this pulse?
b) What is the intensity (in W/m2) delivered to the cell?
c) What are the maximum values of the electric and magnetic fields in the pulse?
To get the field strengths, recall our formulas:
u
2
1

E
2 0

1
20
2
2
B  0E 
1
0
2
B
I
Power
 uc
Area
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Example: High-Energy Cancer Treatment
Scientists are working on a technique to kill cancer cells by zapping them with ultrahighenergy pulses of light that last for an extremely short amount of time. These short pulses
scramble the interior of a cell without causing it to explode, as long pulses do.
We can model a typical such cell as a disk 5.0 µm in diameter, with the pulse lasting for
4.0 ns with an average power of 2.0x1012 W. We shall assume that the energy is spread
uniformly over the faces of 100 cells for each pulse.
a) How much energy is given to the cell during this pulse?
b) What is the intensity (in W/m2) delivered to the cell?
c) What are the maximum values of the electric and magnetic fields in the pulse?
To get the field strengths, recall our formulas:
u
2
1

E
2 0

1
20
2
2
B  0E 
Since the power was stated as
average power we should
assume that is the rms value. So
our field values should get
multiplied by √2 to find the
maximum.
1
0
2
B
I
E
2I
V
 8.7  101 1 m
c  0
B
20  I
 2.9  103 T
c
Power
 uc
Area
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Energy and momentum in EM Waves
EM waves also carry momentum. This means that a ray of light can actually exert a
force. To get the pressure exerted by a sinusoidal EM wave, just divide the intensity
by the speed of light.
Radiation Iav

c
Pr essure
This is the same as the total energy absorbed by the surface.
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Energy and momentum in EM Waves
EM waves also carry momentum. This means that a ray of light can actually exert a
force. To get the pressure exerted by a sinusoidal EM wave, just divide the intensity
by the speed of light.
Radiation Iav

c
Pr essure
Example: Solar Sails
Suppose a spacecraft with a mass of 25,000 kg has a solar sail made of perfectly
reflective aluminized film with an area of 2.59x106 m. If the spacecraft is launched
into earth orbit and then deploys its sail at right angles to the sunlight, what is the
acceleration due to sunlight? Assume that at the earth’s distance from the sun, the
pressure exerted by sunlight on an absorbing surface is 4.70x10-6 Pa.
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Example: Solar Sails
Suppose a spacecraft with a mass of 25,000 kg has a solar sail made of perfectly
reflective aluminized film with an area of 2.59x106 m. If the spacecraft is launched
into earth orbit and then deploys its sail at right angles to the sunlight, what is the
acceleration due to sunlight? Assume that at the earth’s distance from the sun, the
pressure exerted by sunlight on an absorbing surface is 4.70x10-6 Pa.
Recall that Pressure = Force/Area. We can use this and F=ma to get our formula:
F
F PA
A
F
F  ma  a 
m
P
PA
a
m
Now for the tricky part: When the pressure number was given above, that was for
an absorbing surface. What happens when the sunlight reflects instead?
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Example: Solar Sails
Suppose a spacecraft with a mass of 25,000 kg has a solar sail made of perfectly
reflective aluminized film with an area of 2.59x106 m. If the spacecraft is launched
into earth orbit and then deploys its sail at right angles to the sunlight, what is the
acceleration due to sunlight? Assume that at the earth’s distance from the sun, the
pressure exerted by sunlight on an absorbing surface is 4.70x10-6 Pa.
Recall that Pressure = Force/Area. We can use this and F=ma to get our formula:
F
F PA
A
F
F  ma  a 
m
P
PA
a
m
Now for the tricky part: When the pressure number was given above, that was for
an absorbing surface. What happens when the sunlight reflects instead?
Twice as much momentum is transferred!
a
2(4.7  106
N )  2.59  106 m2
m2
4
2.5  10 kg
 9.72  10 4
m
s2
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Polarization
The Polarization of an EM wave is defined to be the direction of its Electric field vector.
EM waves (or light) can be passed through a filter (polarizer) to select for a particular
polarization direction. This will cut down the intensity (brightness) of the light based
on the following formula:
I  I0  cos()
2
Polarizers can be placed in sequence to adjust the intensity and polarization of light.
The most obvious example is dark sunglasses, where 2 filters are placed at 90° to each
other, blocking out most of the light (the formula would say all the light is blocked).
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Polarization
Details about polarization:
Typical light sources are unpolarized, which means the EM waves are not oriented in
any particular direction (sunlight behaves this way). When unpolarized light passes
through a polarizer, half of its intensity is blocked, and the transmitted light is now
polarized in the direction selected by the filter.
Example Problem
• Sunlight passes through 2 polarizers which are oriented at 60° relative to each other.
How much of the original sunlight intensity is transmitted?
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Polarization
Details about polarization:
Typical light sources are unpolarized, which means the EM waves are not oriented in
any particular direction (sunlight behaves this way). When unpolarized light passes
through a polarizer, half of its intensity is blocked, and the transmitted light is now
polarized in the direction selected by the filter.
Example Problem
• Sunlight passes through 2 polarizers which are oriented at 60° relative to each other.
How much of the original sunlight intensity is transmitted?
 

 2
1
Ifinal  Isun 
 cos(60 )  1  Isun
2 
8
1
4
Click this link for a java applet with polarizers.
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Polarization
Details about polarization:
Typical light sources are unpolarized, which means the EM waves are not oriented in
any particular direction (sunlight behaves this way). When unpolarized light passes
through a polarizer, half of its intensity is blocked, and the transmitted light is now
polarized in the direction selected by the filter.
Reflected light is (at least partially) polarized parallel to the reflecting surface. A good
example is sunlight reflecting from the water. Fishermen wear polarized sunglasses to
block the reflected sunlight, giving them a better view of objects beneath the surface.
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