Upload
melvyn-haynes
View
244
Download
1
Embed Size (px)
DESCRIPTION
x z y E B Only the loop in the xy plane will have a magnetic flux through it as the wave passes. The flux will oscillate with time and induce an emf. (Faraday’s Law!) loop in xy plane loop in xz plane loop in yz plane Which orientation will have the largest induced emf? Preflight 15.1, 15.2
Citation preview
Physics 102: Lecture 15, Slide 1
Electromagnetic Wavesand Polarization
• Today’s lecture will cover Textbook Sections 22.7-8
Physics 102: Lecture 15
Physics 102: Lecture 15, Slide 2
xz
yE
B
loop in xy plane
loop in xz plane
loop in yz
plane
1 2 3
Which orientation will have the largest induced emf? Hint: Loops use B not E.
Preflight 15.1, 15.2
xz
yE
B
Only the loop in the xy plane will have a magnetic flux through it as the wave passes. The flux will oscillate with time and induce an emf. (Faraday’s Law!)
loop in xy plane
loop in xz plane
loop in yz
plane
1 2 3
Which orientation will have the largest induced emf?
Preflight 15.1, 15.2
Physics 102: Lecture 15, Slide 4
Propagation of EM Waves
• Changing B field creates E field• Changing E field creates B field
E = c B
xz
y
If you decrease E, you also decrease B!
This is important !
Physics 102: Lecture 15, Slide 5
Preflight 15.4
Suppose that the electric field of an electromagnetic wave decreases in magnitude. The magnetic field: 1 increases
2 decreases
3 remains the same
Physics 102: Lecture 15, Slide 6
Preflight 15.4
Suppose that the electric field of an electromagnetic wave decreases in magnitude. The magnetic field: 1 increases
2 decreases
3 remains the same
E=cB
Physics 102: Lecture 15, Slide 7
Energy in EM waveLight waves carry energy but how?
Electric Fields • Recall Capacitor Energy:
U = ½ C V2
• Energy Density (U/Volume): uE = ½ 0E2
• Average Energy Density: uE = ½ (½ 0E0
2)
= ½ 0E2rms
Magnetic Fields • Recall Inductor Energy:
U = ½ L I2
• Energy Density (U/Volume):uB = ½ B2/0
• Average Energy Density: uB = ½ (½ B0
2/0)
= ½ B2rms/0
Physics 102: Lecture 15, Slide 8
Energy Density
Calculate the average electric and magnetic energy density of sunlight hitting the earth with Erms = 720 N/C
202
1rmsE Eu
0
2
21
rms
BBu
00
1
c
Note: This is true only for EM waves.
Energy Density
Calculate the average electric and magnetic energy density of sunlight hitting the earth with Erms = 720 N/C
202
1rmsE Eu
2212
2
1 C N8.85 10 720 2 Nm C
0
2
21
rms
BBu 2
0
2
21
cErms
00
1
cUse
ErmsB uEu 202
1 36106.42
mJuuuu EBEtotal
Note: This is true only for EM waves.
63
J2.3 10m
Physics 102: Lecture 15, Slide 10
Energy in EM waveElectric and magnetic fields carry equal amounts of energy.
Electric Fields • Average Energy Density:
uE = ½ (½ 0E02)
= ½ 0E2rms
Magnetic Fields
• Average Energy Density: uB = ½ (½ B0
2/0)
= ½ B2rms/0
= ½ E2rms/(c20)
= ½ 0E2rms
In EM waves, E field energy = B field energy! ( uE = uB )
Physics 102: Lecture 15, Slide 11
Intensity (I or S) = Power/Area• Energy (U) in box:
U = u x Volume = u (AL)
• Power (P):
L
A
L=ct
P = U/t = U (c/L) = u A c
• Intensity (I or S): S = P/A = uc = c0E2
rms23
U = Energy u = Energy Density (Energy/Volume)A = Cross section Area of lightL = Length of box 23
Physics 102: Lecture 15, Slide 12
Polarization• Transverse waves have a polarization
– (Direction of oscillation of E field for light)• Types of Polarization
– Linear (Direction of E is constant)– Circular (Direction of E rotates with time)**
– Unpolarized (Direction of E changes randomly)
xz
y
Physics 102: Lecture 15, Slide 13
Linear Polarizers• Linear Polarizers absorb all electric fields
perpendicular to their transmission axis.
Molecular View (link)
Unpolarized Light on Linear Polarizer
• Most light comes from electrons accelerating in random directions and is unpolarized.
• Averaging over all directions: Stransmitted= ½ Sincident
Always true for unpolarized light!
Physics 102: Lecture 15, Slide 15
Linearly Polarized Light on Linear Polarizer (Law of Malus)
Etranmitted =Stransmitted =
TA
is the angle between the incoming light’s polarization, and the transmission axis
Transmission axisIncident E
ETransmitted
Eabsorbed
=Eincidentcos()
Physics 102: Lecture 15, Slide 16
Linearly Polarized Light on Linear Polarizer (Law of Malus)
Etranmitted = Eincident cos()Stransmitted = Sincident cos2()
TA
is the angle between the incoming light’s polarization, and the transmission axis
Transmission axisIncident E
ETransmitted
Eabsorbed
=Eincidentcos()
Physics 102: Lecture 15, Slide 17
Preflight 15.6, 15.7Unpolarized light (like the light from the sun) passes through a polarizing sunglass (a linear polarizer). The intensity of the light when it emerges is 1. zero
2. ½ what it was before 3. ¼ what it was before 4. ⅓ what it was before 5. need more information
Now, horizontally polarized light passes through the same glasses (which are vertically polarized). The intensity of the light when it emerges is
1. zero2. ½ what it was before3. ¼ what it was before4. ⅓ what it was before5. Need more information
Physics 102: Lecture 15, Slide 18
Preflight 15.6
Unpolarized light (like the light from the sun) passes through a polarizing sunglass (a linear polarizer). The intensity of the light when it emerges is
1. zero 2. 1/2 what it was before 3. 1/4 what it was before 4. 1/3 what it was before 5. need more information
Physics 102: Lecture 15, Slide 19
Preflight 15.7
Now, horizontally polarized light passes through the same glasses (which are vertically polarized). The intensity of the light when it emerges is
• zero • 1/2 what it was before • 1/4 what it was before • 1/3 what it was before • need more information
Physics 102: Lecture 15, Slide 20
Law of Malus – 2 Polarizers
S1 =
S2 =
unpolarized light
E1
I = I0
TATA
TA
E0
I3
B1
unpolarized light
E1
I = I0
TATA
TA
E0
I3
B1S = S0
S1
S2
Physics 102: Lecture 15, Slide 21
Law of Malus – 2 Polarizers
Cool Link
unpolarized light
E1
I = I0
TATA
TA
E0
I3
B1
unpolarized light
E1
I = I0
TATA
TA
E0
I3
B1
1) Intensity of unpolarized light incident on linear polarizer is reduced by ½ . S1 = ½ S0
S = S0 S1
S2
2) Light transmitted through first polarizer is vertically polarized. Angle between it and second polarizer is =90º. S2 = S1 cos2(90º) = 0
Physics 102: Lecture 15, Slide 22
unpolarized light
E1
I = I0
TATA
TA
E0
I3
B1
unpolarized light
E1
I = I0
TATA
TA
E0
I3
B1
Law of Malus – 3 Polarizers
I2 =
I3 =
I1 =
unpolarized light
E1
I = I0
TATA
TA
E0
I3
B1
unpolarized light
E1
I = I0
TATA
TA
E0
I3
B1
Law of Malus – 3 Polarizers
2) Light transmitted through first polarizer is vertically polarized. Angle between it and second polarizer is =45º. I2 = I1 cos2 (45º) = ½ I0 cos2 (45º)
3) Light transmitted through second polarizer is polarized 45º from vertical. Angle between it and third polarizer is =45º. I3 = I2 cos2 (45º)
I2= I1cos2(45)
= ½ I0 cos4 (45º)
I1= ½ I0
Physics 102: Lecture 15, Slide 24
TA
TA
S1
S2
S0
TATA
S1
S2
S0
ACT: Law of Malus
A B
1) S2A > S2
B 2) S2A = S2
B
3) S2A < S2
B
E0E0
Physics 102: Lecture 15, Slide 25
TA
TA
S1
S2
S0
TATA
S1
S2
S0
ACT: Law of Malus
A B
1) S2A > S2
B 2) S2A = S2
B
3) S2A < S2
B
S1= S0cos2(60)
S2= S1cos2(30)= S0 cos2(60) cos2(30)
S1= S0cos2(60)
S2= S1cos2(60)= S0 cos4(60)
Cool Link
E0E0
Physics 102: Lecture 15, Slide 26
See next time!• Read Sections 23.1-2, 7-8