Electromagnetic Waves

From radio waves to gamma rays - the electromagnetic spectrum and how light behaves as a wave.

All Topics

Wavelength ↔ Frequency Calculator

Formula
c = fλ → f = c/λ
Wavelength
nm
Result
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1 The Electromagnetic Spectrum

All electromagnetic waves travel at c = 3 × 10⁸ m/s in vacuum but differ in wavelength and frequency. From longest to shortest wavelength: radio → microwave → infrared → visible → ultraviolet → X-ray → gamma ray.

Radio
λ > 1 m, f < 300 MHz
Microwave
1 mm – 1 m, WiFi/5G/radar
Infrared
700 nm – 1 mm, heat/thermal
Visible
400–700 nm (violet→red)
Ultraviolet
10–400 nm, sunburn
X-ray
0.01–10 nm, medical imaging
Gamma
< 0.01 nm, nuclear decay
c = fλ
c = 3 × 10⁸ m/s, f = frequency (Hz)λ = wavelength (m)Higher frequency = shorter wavelength = more energy
Worked Example 1

WiFi Signal Wavelength

Problem: Your WiFi router broadcasts at 5.0 GHz. What is the wavelength? What part of the EM spectrum is this?
Apply c = fλ
λ = c/f = 3×10⁸ / 5.0×10⁹
λ = 0.06 m = 6 cm (microwave)
Answer: 6 cm wavelength - microwave range. This is why WiFi can be blocked by walls (wavelength comparable to gaps) and why microwave ovens operate at similar frequencies (2.45 GHz, λ = 12.2 cm).

2 Maxwell's Equations - The Complete Theory

James Clerk Maxwell unified electricity, magnetism, and optics into four elegant equations that describe all electromagnetic phenomena. They predict that changing electric fields create magnetic fields and vice versa - together forming self-propagating waves at the speed of light.

Gauss (E)
∇·E = ρ/ε₀ (charges create E fields)
Gauss (B)
∇·B = 0 (no magnetic monopoles)
Faraday
∇×E = −∂B/∂t (changing B creates E)
Ampère-Maxwell
∇×B = μ₀J + μ₀ε₀∂E/∂t

3 Wave Properties - Interference & Diffraction

EM waves exhibit interference (constructive when crests align, destructive when crest meets trough) and diffraction (bending around obstacles or through slits). These wave behaviors prove light is a wave - complementing its particle nature (wave-particle duality).

Young's Double Slit: d sin θ = mλ
d = slit separation, θ = angle to bright fringem = 0, ±1, ±2... (fringe order)Bright fringes where path difference = whole wavelengths
Worked Example 2

Double Slit Experiment

Problem: Light of wavelength 600 nm passes through two slits 0.2 mm apart. A screen is 2 m away. What is the spacing between bright fringes?
Fringe spacing formula
Δy = λL/d = (600×10⁻⁹ × 2) / (0.2×10⁻³)
Δy = 6.0 × 10⁻³ m = 6.0 mm
Answer: 6.0 mm between bright fringes. Longer wavelength → wider spacing. Narrower slits → wider spacing. This experiment was first performed by Thomas Young in 1801, proving light is a wave.

4 Polarization

Light is a transverse wave - the electric field oscillates perpendicular to the direction of travel. Unpolarized light has E oscillating in all perpendicular directions. A polarizer transmits only one direction. Two perpendicular polarizers block all light.

Malus's Law: I = I₀ cos²θ
I₀ = intensity after first polarizerθ = angle between polarizer axesAt 90°: I = 0 (crossed polarizers)
Worked Example 3

Malus's Law - Polarizer Angle

Problem: Unpolarized light passes through two polarizers. The second is at 30° to the first. What fraction of the original intensity passes through?
Two-stage reduction
After 1st polarizer: I₁ = I₀/2 (always halves unpolarized)
After 2nd: I₂ = I₁ cos²(30°) = (I₀/2)(√3/2)² = (I₀/2)(3/4)
I₂ = 3I₀/8 = 0.375 I₀ (37.5%)
Answer: 37.5% of original intensity. At 45° it would be 25%, at 60° only 12.5%, at 90° zero. Polarized sunglasses work by blocking horizontally polarized glare from reflective surfaces.

5 Electromagnetic Wave Energy

EM waves carry energy described by the Poynting vector. The intensity (power per area) is proportional to the square of the electric field amplitude.

I = P/A = ½cε₀E₀²
I = intensity (W/m²)E₀ = peak electric field (V/m)Sun at Earth: I ≈ 1361 W/m² → E₀ ≈ 1013 V/m

6 Inverse Square Law & Radiation

EM radiation spreads over an expanding sphere. Intensity decreases with the square of distance from the source.

I = P / (4πr²)
Double the distance → ¼ the intensityTriple the distance → 1/9 the intensity
Why stars are dim: The Sun's luminosity is 3.85 × 10²⁶ W. At Earth (1.5 × 10¹¹ m away): 1,361 W/m². At Pluto: only 0.9 W/m². At the nearest star (4.24 ly): 3 × 10⁻⁸ W/m².
The Electromagnetic Spectrum γ-rays X-rays UV Visible IR Microwave Radio ← higher frequency, higher energy, shorter wavelength

Wave Speed / Period Calculator

Formulas
c = fλ | T = 1/f
f Frequency (Hz)
Wavelength | Period
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Snell's Law Calculator

Formula
n₁ sin θ₁ = n₂ sin θ₂
n₁ Refractive index medium 1
θ₁ Angle of incidence (°)
n₂ Refractive index medium 2
Angle of Refraction (θ₂)
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