
Physics II course sequence · Interactive lesson
Electromagnetic spectrum & polarization
The wave solution fixes the speed and the geometry, then leaves two labels free: how fast the field oscillates, and which way it points across the beam. Those two labels sort every source, every interaction and every hazard you will meet.
UPII-12.08 · Lesson 8 of 8 in this unit. Position is not a completion score.Build the model
One wave equation, fifteen decades of frequency, two transverse directions.
The key idea
The electromagnetic spectrum is the continuous range of frequencies a transverse electromagnetic wave can carry, and its polarization state is the pattern traced by E in the plane across the direction of travel.
Example. Green light at f = 5.6 × 10¹⁴ Hz has λ = c/f = 535 nm and a photon energy hf = 2.32 eV; if E stays on one fixed line, a polarizer turned 60° from that line passes cos²60° = 25% of the intensity.
The complete physical model and assumptions
Every electromagnetic wave you will meet is the same solution wearing two different labels, and this topic is about reading both. The first label is frequency. Nothing in the wave equation prefers one value, so the same transverse solution runs continuously from kilohertz radio to 10²⁰ Hz gamma rays, with c = f λ tying the two names for a band together. What changes across that range is not the wave but the matter it meets: a material responds when the drive lands near one of its own frequencies, which means molecular rotation in the microwave, bond vibration in the infrared, valence-electron transitions through the visible and ultraviolet, and core electrons and nuclei above. The second label is the direction of E in the plane across the beam. Because E and B are both perpendicular to the propagation direction, that plane is two-dimensional, and the relative amplitude and phase of its two components define the polarization state: linear, circular or elliptical, with ordinary thermal light an incoherent churn through all of them. A polarizer projects one component out, and Malus's law is that projection squared. Where the model gives out is set by the photon energy E = hf: the classical field describes propagation beautifully at every frequency, but it cannot say why one ultraviolet quantum breaks a bond while a kilowatt of radio only warms.
1Frequency is the label the wave equation leaves free
Derive the wave equation from Maxwell's equations and out drops a single speed, c = 1/√(ε₀μ₀), together with a fixed geometry in which E, B and the propagation direction are mutually perpendicular. No frequency appears anywhere in that derivation. Any f solves the equations, so the spectrum is continuous and the band names are human conventions laid over it. In vacuum c = f λ converts between them: 1.0 MHz is 300 m, 2.45 GHz is 12.2 cm, 1.0 × 10¹³ Hz is 30 μm, 5.0 × 10¹⁴ Hz is 600 nm, 1.0 × 10¹⁸ Hz is 0.30 nm. Notice the scale. From long-wave radio near 10⁵ Hz to gamma rays above 10²⁰ Hz is fifteen decades, and the visible band, 400 nm to 700 nm, is less than one octave inside it. Note also that λ depends on the medium while f does not: light entering glass of index 1.50 keeps its frequency, because the driven charges oscillate at the drive frequency, and shortens its wavelength to λ/1.50.
2What a band does is set by what resonates with it
A band is characterised by the motion it can drive, and matter responds strongly only when the drive lands near one of its own frequencies. Radio moves free electrons along conductors, which is why an efficient antenna is a fraction of a wavelength long. Microwaves at 2.45 GHz push on the permanent dipole of the water molecule faster than the surrounding liquid lets it turn, and the lag dumps energy as heat. Infrared near 10¹³ Hz matches molecular vibration: the bending mode of CO₂ sits at 667 cm⁻¹, which is 2.0 × 10¹³ Hz and λ = 15 μm, the wavelength it removes from outgoing thermal radiation. Visible and ultraviolet quanta of 1.8 eV to 12 eV move valence electrons between levels, which is colour and photochemistry. X-rays reach the core electrons, and at λ ≈ 0.1 nm they diffract from the atomic planes of a crystal.
3Photon energy, not intensity, draws the ionizing line
Rank a band by what one quantum can do and the tool is E = hf, or E = hc/λ with the shortcut hc = 1240 eV nm. Red light at 700 nm is 1.77 eV, violet at 400 nm is 3.10 eV, a 250 nm germicidal line is 4.96 eV, and 124 nm is exactly 10.0 eV. Set those against the energies matter cares about: a C–C bond is about 3.6 eV and the first ionization energy of water is 12.6 eV. That comparison is where the non-ionizing boundary near 10 eV comes from, and it is a per-quantum statement, so intensity cannot move it. A 900 W oven at 2.45 GHz delivers 5.5 × 10²⁶ photons per second, each carrying 1.0 × 10⁻⁵ eV; a 4 W lamp at 250 nm delivers 5.0 × 10¹⁸ per second, each carrying 4.96 eV. The oven has 225 times the power and half a million times less energy per quantum.
4Two directions across the beam, and the states they build
Transversality leaves E free in a two-dimensional plane, so write it in components: E = Eₓ cos(kz − ωt) x̂ + Ey cos(kz − ωt + δ) ŷ. Two amplitudes and one relative phase δ describe every state there is. With δ = 0 the components rise and fall together and the tip of E runs back and forth along a fixed line tilted at arctan(Ey/Eₓ); with δ = π the y component is simply flipped in sign, so the line tilts the other way, at −arctan(Ey/Eₓ). Either value gives linear polarization. With δ = ±π/2 and Eₓ = Ey the tip travels a circle once per period, one way or the other according to the sign: circular polarization. Everything else is an ellipse. Thermal light from a filament or the Sun is none of these for long, because it arrives as an uncorrelated flood from enormous numbers of independent atoms; orientation and δ scramble on a nanosecond timescale, and averaged over any detection time the beam is unpolarized.
5A polarizer projects amplitude, and each one resets the state
An ideal polarizing sheet transmits only the component of E along its transmission axis. Projection acts on amplitude, E = E₀ cosθ, and intensity goes as amplitude squared, which is Malus's law I = I₀ cos²θ. Feed it unpolarized light instead and every orientation occurs equally often; the average of cos²θ over all angles is ½, so the first sheet passes half whichever way it is turned, and what leaves it is polarized along its axis. Chain three sheets and the consequence is sharp. Crossed sheets at 0° and 90° pass nothing. Slide a third sheet at 45° between them and the output is ½ × ½ = ¼ of what left the first sheet, because the middle sheet does not merely subtract: light leaving it is polarized at 45°, and 45° is only 45° away from the analyzer.
6The evidence for transversality, and where the model gives out
Polarization is itself the evidence that the field is transverse. A longitudinal wave has no direction to choose across its line of travel, which is why sound cannot be polarized, and why rotating a sheet about the beam axis could never change what passes if E lay along the propagation direction. Two everyday effects confirm it. Light reflected near Brewster's angle, tan θB = n₂/n₁, which is 56.3° for air on glass of index 1.50, is strongly polarized parallel to the surface, and polarized sunglasses live on that fact. Sunlight scattered through 90° in the sky is polarized too, because the driven air molecules radiate nothing along their own oscillation direction. Two limits bound the model: real sheets absorb, so a Polaroid passes about 38% of unpolarized light rather than 50%, and no wave picture explains why absorption arrives in quanta of hf.
Key equations
Read the units, assumptions and limits before substituting.
Frequency and wavelength in vacuum
c = f λ
Converts a band named by wavelength into the same band named by frequency.
f in Hz, λ in m, c = 2.998 × 10⁸ m s⁻¹; in a medium of index n, λ shortens to λ/n while f is unchangedPhoton energy
E = h f = h c / λ
Ranks a band by what one quantum can do, which no intensity tells you.
h = 6.626 × 10⁻³⁴ J s, E in J; 1 eV = 1.602 × 10⁻¹⁹ J, and hc = 1240 eV nmMalus's law
I = I₀ cos²θ
Turns an angle into a transmitted fraction, since the sheet passes a component of amplitude.
I₀ and I in W m⁻²; θ is the angle from the incoming polarization to the transmission axisUnpolarized light through the first sheet
I₁ = ½ Iᵤₙₚₒₗ
The average of cos²θ over all orientations is ½, a fixed toll paid once.
Intensities in W m⁻². Independent of how the sheet is turned; the output is polarized along its axisPolarization state of a transverse wave
E = Eₓ cos(kz − ωt) x̂ + Ey cos(kz − ωt + δ) ŷ
δ = 0 or π gives linear; δ = ±π/2 with Eₓ = Ey gives circular; else elliptical.
Eₓ, Ey in V m⁻¹; δ is the relative phase of the two components, in rad, and with the sign convention written here a positive δ delays the y componentBrewster's angle
tan θB = n₂ / n₁
The one incidence angle at which the reflected beam is fully polarized.
θB measured from the normal; n₁, n₂ dimensionless refractive indices, 56.3° for air on glass of index 1.50Interactive lab
Predict first. Explore the model. Compare the result.
Explore the model
Try this. Park the analyzer at 90°, where the third readout says a bare crossed pair passes nothing, then drag P₂ from 0° up to 45° and watch a quarter of the light reappear. Each sheet re-prepares the state instead of filtering a fixed one.
Live results
- AFTER P₂ I₂ / I₁
- 0.750
- AFTER P₃ I₃ / I₁
- 0.188
- P₂ REMOVED I₃ / I₁
- 0.000
- ANGLE FROM P₂ TO P₃
- 60 °
Results follow this lesson’s model and assumptions. Displayed values are rounded.
Predict → change one variable → check
Plan a change before running it. Every other input stays at the saved baseline.
Saved baseline. Middle sheet P₂ angle: 30 °; Analyzer P₃ angle: 90 °
This experiment is kept only while this page is open. It does not change saved course progress.
Catch the common trap
A polarizer is not a sieve that strains out the light pointing the wrong way. It projects: the component of E along its axis passes with amplitude E₀ cosθ, the perpendicular component is absorbed, and what emerges is polarized along the sheet's axis whatever it was before. Treating the sheet as a filter makes the three-sheet result look impossible — if two crossed sheets pass nothing, how can a third sheet inserted between them pass a quarter? A filter can only remove; a projector re-prepares. The middle sheet at 45° hands the analyzer light polarized at 45°, not the original 0° light with a slice missing. The same error breeds the belief that the ½ for unpolarized light means half the photons were already aligned. Every photon is projected, and the average of cos²θ over all orientations is ½.
Practice & worked examples
3 authored examples. Make an attempt, then reveal the reasoning one step at a time.
EasyExample 1
An FM station broadcasts on 98.5 MHz. Find the wavelength in air, the length of a quarter-wave whip antenna tuned to it, and the energy of one photon in both joules and electronvolts.
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 4 steps revealed.
- Air is close enough to vacuum for radio, so λ = c/f = 2.998 × 10⁸ m s⁻¹ ÷ 9.85 × 10⁷ Hz = 3.0437 m, or 3.04 m to three significant figures.
- A quarter-wave whip is λ/4 = 3.0437/4 = 0.761 m, which is why car aerials are that length rather than metres long — the antenna is sized by the wavelength, not by the frequency number.
- Photon energy: E = hf = 6.626 × 10⁻³⁴ J s × 9.85 × 10⁷ Hz = 6.53 × 10⁻²⁶ J.
- In electronvolts, E = 6.527 × 10⁻²⁶ ÷ 1.602 × 10⁻¹⁹ = 4.07 × 10⁻⁷ eV — about ten million times smaller than the 3.6 eV of a chemical bond, so this radiation can shake charges but never rearrange them.
Answer. λ = 3.04 m, quarter-wave whip 0.761 m, photon energy 6.53 × 10⁻²⁶ J = 4.07 × 10⁻⁷ eV.
MediumExample 2
Unpolarized light of intensity 240 W m⁻² reaches a polarizing sheet, and a second sheet stands with its axis 65° from the first. Find the intensity after each sheet, then find the angle to which the second sheet must be turned so that 30 W m⁻² emerges.
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 5 steps revealed.
- The first sheet meets unpolarized light, so it passes half regardless of orientation: I₁ = ½ × 240 = 120 W m⁻², now polarized along its own axis.
- That light is polarized, so the second sheet obeys Malus's law with θ = 65°: cos 65° = 0.4226, and cos²65° = 0.1786.
- I₂ = 120 × 0.1786 = 21.4 W m⁻².
- For 30 W m⁻² the required fraction is cos²θ = 30/120 = 0.250, so cos θ = 0.500 and θ = 60.0°.
- Check the direction of the change: 60° is closer to alignment than 65°, so more light should pass — and 30 W m⁻² is indeed more than 21.4 W m⁻².
Answer. I₁ = 120 W m⁻², I₂ = 21.4 W m⁻²; turning the second sheet to 60.0° from the first gives 30 W m⁻².
HardExample 3
Unpolarized light of intensity 480 W m⁻² passes through P₁, then a sheet P₂ whose axis is φ from P₁, then an analyzer P₃ crossed at 90° to P₁. Write the transmitted intensity as a function of φ, find the φ that maximizes it and that maximum, then compare it with a stack whose two middle sheets sit at 30° and 60°.
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 6 steps revealed.
- P₁ halves the unpolarized beam: I₁ = 240 W m⁻², polarized along the P₁ axis.
- P₂ is at φ from that polarization, and P₃ is then at 90° − φ from the polarization leaving P₂, so I₃ = 240 cos²φ cos²(90° − φ) = 240 cos²φ sin²φ W m⁻².
- Use sin φ cos φ = ½ sin 2φ to fold it into one term: I₃ = 240 × ¼ sin²2φ = 60.0 sin²2φ W m⁻².
- sin²2φ peaks at 1 when 2φ = 90°, so φ = 45.0° and I₃ = 60.0 W m⁻² — one quarter of I₁, from a pair that passed nothing before P₂ was inserted.
- Now two middle sheets at 30° and 60°: each step is 30°, so I = 240 × (cos²30°)³ = 240 × 0.750³ = 101 W m⁻².
- The pattern: N equal steps of (90/N)° give I₁ cos(2N)(90/N)°, which rises towards I₁ as N grows — each extra sheet costs a small factor but shrinks every step, so the polarization can be dragged through 90° at almost no cost.
Answer. I₃ = 60.0 sin²2φ W m⁻², maximum 60.0 W m⁻² at φ = 45.0°; with middle sheets at 30° and 60° the output rises to 101 W m⁻².
Quick check
Select an answer and explain it before checking.
Review & continue
The electromagnetic spectrum is the continuous range of frequencies a transverse electromagnetic wave can carry, and its polarization state is the pattern traced by E in the plane across the direction of travel.
- Explain the relationship without looking at the equation.
- Check a sign, a unit and a model assumption in your working.
- Return to the lab or worked example if a step is still unclear.
Optional supporting lessons
These chapter resources can help with earlier ideas; they are not additional required Physics II completion tasks.