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Spec mapping: OCR H556 Module 4.4 — Waves: polarisation as restriction to a single plane; only transverse waves can be polarised; Malus's law I=I0cos2θ; PAG 3 anchor (polarisation). (Refer to the official OCR H556 specification document for exact wording.)
Polarisation is arguably the subtlest of the basic wave phenomena. It is also one of the most powerful pieces of experimental evidence for the transverse nature of light, and it has genuine practical applications — from sunglasses and camera filters to LCD screens and 3D cinema. The OCR A-Level Physics A specification asks you to understand what polarisation is, why only transverse waves can be polarised, how polarising filters (like Polaroid) work, and — in the OCR context uniquely among the A-Level boards — to apply Malus's law:
I=I0cos2θ
This is the equation you must memorise and be able to deploy. The rest of this lesson establishes the physical content behind it.
In an unpolarised transverse wave, the direction of oscillation changes rapidly and randomly — there is no preferred plane. Natural light from the Sun or from a filament bulb is unpolarised: the electric field vector oscillates in all directions perpendicular to the direction of propagation, changing direction millions of times per second.
A polarised transverse wave is one in which the oscillation is restricted to a single plane containing the direction of propagation. That plane is called the plane of polarisation (OCR's convention is to define this as the plane containing the electric field vector and the direction of propagation).
Only transverse waves can be polarised, because only transverse waves have oscillations in multiple possible directions perpendicular to propagation. Longitudinal waves (like sound) oscillate only along the direction of travel — there is nothing left to restrict, so polarisation is meaningless for them.
This is the crucial experimental evidence that light is transverse: by 1808, Étienne-Louis Malus had observed that a beam of light reflected off glass at certain angles could be partially blocked by a second piece of glass oriented perpendicular to the first. Something about the reflected light made it asymmetric about the direction of travel — and that could only happen for a transverse wave.
A polarising filter (commonly called a Polaroid filter, after the commercial product invented by Edwin Land in 1929) contains long-chain conducting molecules all aligned in the same direction. These chains absorb the component of the electric field parallel to them, transmitting only the component perpendicular to them.
The direction along which the filter transmits is called its transmission axis.
flowchart LR
U[Unpolarised light: E vibrates in all directions] --> F1[Polariser: transmission axis vertical]
F1 --> P[Vertically polarised light: amplitude reduced by sqrt 2]
P --> F2[Analyser at angle theta]
F2 --> O[Transmitted light: amplitude A cos theta, intensity I cos squared theta]
When unpolarised light of intensity I0 passes through a single polariser, the filter transmits only the component along its transmission axis. Since the incoming light is random in orientation, averaging cos2θ uniformly over all directions gives ⟨cos2θ⟩=1/2, so only half the intensity is transmitted:
I1=2I0
This is the starting point of any polarisation problem.
Once light has been polarised by a first filter (the polariser), you can analyse it with a second filter (the analyser). If the analyser's transmission axis makes an angle θ with the plane of polarisation of the incoming light, the transmitted intensity is given by Malus's law:
I=I0cos2θ
where I0 is the intensity of the already polarised light incident on the analyser, I is the intensity of the light transmitted through the analyser, and θ is the angle between the analyser's transmission axis and the plane of polarisation of the incoming polarised light.
The analyser transmits the component of the electric field along its transmission axis. If the incoming polarised light has electric field amplitude E0 at angle θ to the transmission axis, then the transmitted amplitude is:
E=E0cosθ
But intensity is proportional to the square of the amplitude:
I∝E2⇒I=I0cos2θ
The squaring is why cosθ appears in amplitude equations but cos2θ appears in intensity equations. Be vigilant about this distinction. It is the single most common slip in OCR Malus questions.
Exam Tip: OCR is one of the few A-Level Physics specifications that names Malus's law explicitly and asks you to apply it. Be ready for a worked calculation in which you must identify θ correctly and compute I=I0cos2θ.
| θ | cos2θ | I/I0 | Interpretation |
|---|---|---|---|
| 0° | 1 | 1 | Full transmission — analyser aligned with polariser |
| 30° | 0.75 | 3/4 | Mostly transmitted |
| 45° | 0.5 | 1/2 | Half transmitted |
| 60° | 0.25 | 1/4 | One quarter transmitted |
| 90° | 0 | 0 | Crossed — no light transmitted |
The last row is worth dwelling on: when the analyser is oriented perpendicular to the polariser (crossed polarisers), no light gets through at all. This is the definitive test for whether light is polarised — if rotating the second filter through 90° extinguishes the light, the light was polarised. Conversely, if rotating the second filter changes the brightness but does not extinguish it, the incident light was unpolarised.
Q. Unpolarised light of intensity 200 W m−2 is incident on a polarising filter. Calculate the transmitted intensity.
A. For unpolarised incident light, a single polariser transmits half the intensity:
I=2I0=2200=100 W m−2
Q. Unpolarised light of intensity 800 W m−2 passes first through a polariser, then through an analyser whose transmission axis is at 30° to that of the polariser. Calculate the final transmitted intensity.
A. After the first filter the light is polarised with intensity:
I1=2I0=2800=400 W m−2
This light is now polarised. Applying Malus's law for the second filter:
I2=I1cos2(30°)=400×(23)2=400×0.75=300 W m−2
Q. Polarised light of intensity 60 W m−2 passes through an analyser and emerges with intensity 15 W m−2. Calculate the angle between the light's plane of polarisation and the analyser's transmission axis.
A. Using I=I0cos2θ:
cos2θ=I0I=6015=0.25 cosθ=0.5⇒θ=60°
Q. Unpolarised light of intensity I0 passes through three polarisers in succession. The second is at 45° to the first, and the third is at 90° to the first. Calculate the final transmitted intensity.
A.
This is a famous counter-intuitive result: inserting a filter increases the transmitted intensity (from 0 with just polarisers 1 and 3 crossed, to I0/8 when filter 2 is inserted between them). Each polariser projects the light onto a new axis, gradually "rotating" the plane of polarisation. The physical content: a polariser is not a passive blocker but an active projector.
Q. Polarised light of intensity 40 W m−2 passes through an analyser whose transmission axis is rotated by 20° from the light's plane of polarisation. The transmitted light then passes through a second analyser, whose transmission axis is rotated by another 20° in the same sense. Calculate the final transmitted intensity.
A. Each analyser projects through the same angle of 20°:
After analyser 1: I1=40×cos220°=40×0.883=35.3 W m−2.
After analyser 2: the light leaving analyser 1 is polarised along analyser 1's axis. The angle between this and analyser 2's transmission axis is again 20°, so:
I2=35.3×cos220°=35.3×0.883=31.2 W m−2.
Total cos420° factor: cos4(20°)=(0.940)4≈0.780. In general, N polarisers each separated by θ from the previous one transmit a fraction cos2Nθ of the originally polarised beam — provided the rotations accumulate in the same sense. For small θ this approaches (1−θ2)N≈e−Nθ2, which is the adiabatic-rotation limit familiar from quantum mechanics.
Besides polarising filters, there are several natural ways to produce polarised light.
Light reflected off a non-metallic surface (water, glass, a wet road) is partially polarised parallel to the reflecting surface. At a specific angle — Brewster's angle — the reflected light is completely polarised.
This is why polarising sunglasses work so well for reducing glare: their transmission axis is vertical, so they block the horizontally polarised light reflected off horizontal surfaces like water or roads.
Exam Tip: OCR will ask why polarising sunglasses reduce glare more effectively than ordinary tinted sunglasses. Your answer should mention that light reflected off horizontal surfaces is partially polarised horizontally, and that vertically transmitting sunglasses block this reflected light while still allowing direct (unpolarised) scene light through.
Sunlight scattered off molecules in the atmosphere (Rayleigh scattering) is partially polarised. If you look at a blue sky with a polarising filter and rotate it, the sky will alternately brighten and darken. Bees and other insects can use this atmospheric polarisation pattern to navigate.
Already covered above. This is the most direct laboratory method of producing polarised light and is how polarisation is demonstrated in school.
A standard A-Level laboratory demonstration uses microwaves, listed in OCR's Practical Activity Group 3 (Waves) as the canonical polarisation experiment. A microwave transmitter emits vertically polarised waves (the antenna sets the orientation). If a grid of parallel wires is placed in front of the receiver:
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