Malus's law: Intensity through polarizer:
I=I0cos2θ
where θ is angle from polarization axis.
Electromagnetic Spectrum
All EM waves travel at c in vacuum, differ only in frequency/wavelength:
Radio waves: f<109 Hz
Microwaves: 109 - 1012 Hz
Infrared: 1012 - 1014 Hz
Visible: 4×1014 - 7×1014 Hz
Ultraviolet: 1015 - 1017 Hz
X-rays: 1017 - 1019 Hz
Gamma rays: f>1019 Hz
Standing EM Waves
Boundary conditions (e.g., in cavity) create standing waves:
Ey=2E0sin(kx)cos(ωt)
Nodes:E=0 at x=0,λ/2,λ,...
Used in:
Lasers
Microwave ovens
Radio antennas
Doppler Effect
Source moving with velocity v:
Moving toward observer:f′=fc−vc
Moving away:f′=fc+vc
For v≪c:
fΔf≈cv
📚 Practice Problems
1Problem 1medium
❓ Question:
A plane electromagnetic wave in vacuum has electric field amplitude E₀ = 600 V/m and frequency f = 5.0 × 10¹⁴ Hz. Find: (a) the magnetic field amplitude B₀, (b) the wavelength λ, and (c) the intensity I of the wave.
💡 Show Solution
Given:
E₀ = 600 V/m
f = 5.0 × 10¹⁴ Hz
c = 3.0 × 10⁸ m/s
μ₀ = 4π × 10⁻⁷ T·m/A
ε₀ = 8.85 × 10⁻¹² F/m
(a) Magnetic field amplitude:
In EM waves: E0=cB0
B0=cE0
B0=2.0×10−6 T
(b) Wavelength:
λ=fc=5.0×1
λ=6.0×10−7 m=600 nm
This is orange/yellow visible light!
(c) Intensity:
I=21ε0cE
I=21(8.85×10
I=21(8.85×10
I=477 W/m2
Alternatively: I=2μ0 W/m² ✓
2Problem 2hard
❓ Question:
A laser beam with intensity I = 1.0 × 10⁴ W/m² is incident normally on a perfectly reflecting mirror of area A = 2.0 cm². Find: (a) the radiation pressure on the mirror, (b) the force on the mirror, and (c) compare this to the force if the mirror were perfectly absorbing.
💡 Show Solution
Given:
I = 1.0 × 10⁴ W/m²
A = 2.0 cm² = 2.0 × 10⁻⁴ m²
c = 3.0 × 10⁸ m/s
Perfectly reflecting
(a) Radiation pressure (reflecting):
For perfect reflection:
P=
3Problem 3hard
❓ Question:
A plane EM wave traveling in the +x direction has electric field E= where E₀ = 300 V/m, k = 1.0 × 10⁷ m⁻¹, and ω = 3.0 × 10¹⁵ rad/s. Find: (a) the magnetic field vector, (b) verify these satisfy v = ω/k = c, and (c) the Poynting vector and its time-averaged value.
Wave equations from Maxwell's equations, properties of EM waves
How can I study Electromagnetic Waves effectively?▾
Start by reading the study notes and working through the examples on this page. Then use the flashcards to test your recall. Practice with the 3 problems provided, checking solutions as you go. Regular review and active practice are key to retention.
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What course covers Electromagnetic Waves?▾
Electromagnetic Waves is part of the AP Physics C: Electricity & Magnetism course on Study Mondo, specifically in the Maxwell's Equations section. You can explore the full course for more related topics and practice resources.
Are there practice problems for Electromagnetic Waves?▾
Yes, this page includes 3 practice problems with detailed solutions. Each problem includes a step-by-step explanation to help you understand the approach.
=
3.0×108600
=
2.0
μT
0
14
3.0×108
0
2
−12
)
(
3.0
×
108)(600)2
−12
)
(
3.0
×
108)(3.6×
105)
E0B0
=
2(4π×10−7)(600)(2.0×10−6)=
477
c2I
P=3.0×1082(1.0×104)
P=6.67×10−5 Pa
(b) Force on mirror:
F=PA=(6.67×10−5)(2.0×10−4)
F=1.33×10−8 N=13.3 nN
Very small! But significant for:
Solar sails in space
Optical tweezers (manipulating particles)
Radiation pressure from Sun on comet tails
(c) Perfectly absorbing:
For perfect absorption:
Pabs=cI
Pabs=3.0×1081.0×104=3.33×10−5 Pa
Fabs=(3.33×10−5)(2.0×10−4)
Fabs=6.67×10−9 N=6.67 nN
Reflection produces twice the force as absorption!
Why? Momentum change:
Absorption: Δp = p (from p to 0)
Reflection: Δp = 2p (from +p to -p)
Physics: EM waves carry momentum p=U/c where U is energy
E0sin(kx−
ωt)j^
💡 Show Solution
Given:
E=E0sin(kx−ωt)j^
E₀ = 300 V/m
k = 1.0 × 10⁷ m⁻¹
ω = 3.0 × 10¹⁵ rad/s
Direction: +x
c = 3.0 × 10⁸ m/s
μ₀ = 4π × 10⁻⁷ T·m/A
(a) Magnetic field:
For EM wave: E⊥B direction
E is in +y direction, wave travels in +x, so B must be in ±z direction.
Using right-hand rule (E×B points in propagation direction):
✓