Polarization & Malus's Law

Here is a fact that interference and diffraction, for all their power, could not settle. Both of those effects prove light is a wave — but a wave of what, oscillating in which direction? A sound wave shakes the air back and forth along its own line of travel; a wave on a rope can shake up-and-down or side-to-side, across the direction it runs. Longitudinal or transverse? Interference happens either way, so it stays silent on the question. Polarization is the experiment that breaks the tie, and it answers loudly: light is transverse. Its electric field oscillates strictly across the direction the wave travels, never along it. That single fact has a visible consequence you can hold in your hand. Take two lenses from a pair of polarizing sunglasses, or two squares of Polaroid film, and look through both at a lamp. Rotate one. The light dims, and at one orientation — the two axes at right angles — it goes almost completely black. Nothing has absorbed the light chemically; you have simply asked a transverse wave to squeeze through two gates whose slots are crossed, and a transverse oscillation cannot pass both. Do the same trick with sound and nothing happens at all, because there is no "sideways" to a longitudinal wave to block. This article turns that demonstration into physics. A polarizing filter transmits only the field component along its axis, so unpolarized light loses exactly half its intensity passing the first filter, and then a second filter obeys a clean law discovered by Étienne-Louis Malus in 1809: I=I0cos⁡2θI = I_0\cos^2\theta, where θ\theta is the angle between the two axes. Full through when aligned, half at 45∘45^\circ, dark when crossed. From that one cos⁡2\cos^2 come polarizing sunglasses, LCD screens, photographic filters, and the proof, two centuries old, that light shakes sideways.

Key takeaways
  • Light is a transverse electromagnetic wave: its electric field oscillates perpendicular to the travel direction, so it can be polarized — confined to a single plane.
  • A polarizing filter passes only the field component along its axis. Unpolarized light loses half its intensity through the first filter: I→I0/2I \to I_0/2 (the average of cos⁡2\cos^2 over all angles).
  • A second filter (analyser) at angle θ\theta obeys Malus's law I=I0cos⁡2θI = I_0\cos^2\theta: full at 0∘0^\circ, half at 45∘45^\circ, zero when crossed at 90∘90^\circ.
  • Two crossed filters pass no light — but slip a third filter at 45∘45^\circ between them and light reappears, at Iu/8I_u/8. The order and angles matter.
  • Longitudinal waves (sound) cannot be polarized; polarization is the decisive proof that light is transverse.
  • Key idea: unpolarized light halves through one filter, then a second filter follows I=I0cos⁡2θI = I_0\cos^2\theta — one law that only a transverse wave could obey.
The core insight

Because light is a transverse wave whose electric field can be confined to one plane, a polarizing filter transmits only the field component along its axis: unpolarized light drops to I0/2I_0/2 through the first filter, and a second filter at angle θ\theta then transmits I=I0cos⁡2θI = I_0\cos^2\theta (Malus's law) — full when aligned, zero when crossed.

Where this lives today

The two filters in your polarizing sunglasses are Malus's law you can wear. Glare from a wet road or a lake is light partially polarized by reflection, mostly horizontal; sunglasses set their transmission axis vertical, so cos⁡2θ\cos^2\theta is near zero for that glare and it is cut, while the rest of the scene passes. Every LCD — phone, laptop, television — is a sandwich of two crossed polarizing filters with a liquid-crystal layer between that rotates polarization pixel by pixel, switching each dot between Iu/8I_u/8-style bright and crossed-dark exactly as in the three-filter demonstration. Photographers screw a rotatable polarizing filter onto a lens to deepen skies and kill reflections. Stress engineers shine polarized light through transparent plastic models to see stress patterns light up (photoelasticity), and 3-D cinema hands you glasses whose two lenses are polarized differently so each eye sees its own image. All of it runs on one transverse fact and one cos⁡2\cos^2.

The physical picture

An electromagnetic wave, met earlier in this course, is an oscillating electric field E⃗\vec{E} (with a partner magnetic field) travelling through space. The crucial detail for this article is the direction of that oscillation: E⃗\vec{E} points across the direction of travel — it is a transverse wave. If all the light in a beam happens to oscillate its E⃗\vec{E} in one fixed plane, the light is linearly polarized (or plane-polarized). Ordinary light from the Sun or a lamp is not: it is an incoherent jumble of countless wavetrains from independent atoms, each with its own transverse direction, so the net E⃗\vec{E} points every which way across the beam, changing randomly millions of times a second. That is unpolarized light. A polarizing filter — a Polaroid sheet — has a built-in transmission axis. It behaves like a gate that passes the component of E⃗\vec{E} along that axis and absorbs the component across it. Send polarized light in with its E⃗\vec{E} at angle θ\theta to the axis and only the projection Ecos⁡θE\cos\theta gets through. Send unpolarized light in and, because its direction is random, on average exactly half the intensity survives — the filter keeps one of the two transverse directions and discards the other. After that first filter the light is polarized along the filter's axis, whatever it was before.

Figure
Unpolarized light through two filters — the first halves it to I₀ over 2, the second follows Malus's law with the transmitted intensity depending on the angle θ between the axes
The two-filter chain: halve, then Malus unpolarized intensity I₀ polarizer (axis vertical) polarized I₀/2 analyser (axis at θ) transmitted (I₀/2)cos²θ I₀ → I₀/2 (first filter always halves) → (I₀/2)cos²θ (Malus's law across the angle θ) θ = 0: full · θ = 45°: half · θ = 90°: dark

Unpolarized light through the first filter

Why exactly half? Unpolarized light has its E⃗\vec{E} pointing at every transverse angle ϕ\phi with equal likelihood. Each such component, hitting a filter whose axis is fixed, is itself reduced by cos⁡2ϕ\cos^2\phi (that is Malus's law, which we prove next). To get the transmitted intensity we average cos⁡2ϕ\cos^2\phi over all directions ϕ\phi from 00 to 2π2\pi. The average value of cos⁡2\cos^2 over a full turn is exactly 12\tfrac12, so

I1=I02(1)I_1 = \frac{I_0}{2} \qquad (1)

where: I0I_0 — the incident (unpolarized) intensity; I1I_1 — what survives the first filter, now polarized along its axis. This is not Malus's law with some particular angle — it is the average over all angles, and it is the single most common place students misapply cos⁡2θ\cos^2\theta. Unpolarized light does not have "an angle" to the filter; it has all of them at once, and the average is one half.

Malus's law: the second filter

Now the light is polarized along the first filter's axis with intensity I1I_1. Send it into a second filter — the analyser — whose axis makes angle θ\theta with the first. The analyser passes only the component of the field along its own axis. If the incoming amplitude is E1E_1, the transmitted amplitude is the projection E1cos⁡θE_1\cos\theta. Because intensity is proportional to the square of the amplitude (I∝E2I \propto E^2), the transmitted intensity is

I=I1cos⁡2θ(2)I = I_1\cos^2\theta \qquad (2)

where: θ\theta — the angle between the analyser's axis and the polarization direction of the light reaching it; I1I_1 — the intensity arriving at the analyser. Equation (2) is Malus's law. Read it at the three angles you must know cold: at θ=0\theta = 0 the axes are aligned and I=I1I = I_1 (everything through); at θ=90∘\theta = 90^\circ the axes are crossed and I=0I = 0 (dark); at θ=45∘\theta = 45^\circ, cos⁡245∘=12\cos^2 45^\circ = \tfrac12, so exactly half gets through. The full chain from unpolarized light through two filters is therefore

I=I02cos⁡2θ.(3)I = \frac{I_0}{2}\cos^2\theta. \qquad (3)

The key values, tattooed into every exam: cos⁡230∘=0.75\cos^2 30^\circ = 0.75, cos⁡245∘=0.5\cos^2 45^\circ = 0.5, cos⁡260∘=0.25\cos^2 60^\circ = 0.25, cos⁡290∘=0\cos^2 90^\circ = 0. So a beam already polarized with intensity I1I_1 emerges at 0.75 I10.75\,I_1, 0.5 I10.5\,I_1, 0.25 I10.25\,I_1, and 00 respectively.

Figure
A transverse wave polarized in a single plane, its electric field arrows all vertical, contrasted with unpolarized light whose field points every way across the beam
Transverse light: the electric field oscillates across the travel direction linearly polarized — E confined to one plane all E arrows in one plane → passes a matching filter unpolarized — E points every way across the beam beam coming toward you random transverse directions → filter keeps half sound, being longitudinal, has no across-direction to confine — it cannot be polarized
Derivation AWhy unpolarized light halves and why the analyser follows cos-squared

The goal is to establish both master facts of this topic from one idea — that a filter passes the field component along its axis — giving the half-intensity rule I0/2I_0/2 for the first filter and Malus's law I=I1cos⁡2θI = I_1\cos^2\theta for the second. The strategy is to project the amplitude onto the axis, square it to get intensity, then average over all directions for the unpolarized case. Only algebra and one averaging fact are needed; no calculus is required beyond quoting that the mean of cos⁡2\cos^2 over a full turn is one half.

Step 1. Project the amplitude. Light of amplitude EE whose field makes angle θ\theta with a filter's transmission axis has, along that axis, the component Ecos⁡θE\cos\theta. The filter passes this and absorbs the perpendicular component Esin⁡θE\sin\theta.

Step 2. Square to intensity. Since I∝E2I \propto E^2, the transmitted intensity is I=Iincos⁡2θI = I_{\text{in}}\cos^2\theta, where Iin∝E2I_{\text{in}} \propto E^2 is the incoming intensity. For polarized light entering an analyser at a definite angle θ\theta, this is Malus's law, equation (2).

Step 3. Handle unpolarized input. Unpolarized light is an equal mixture of all directions θ\theta. Each contributes cos⁡2θ\cos^2\theta of its share, so the transmitted fraction is the average of cos⁡2θ\cos^2\theta over 00 to 2π2\pi. Using cos⁡2θ=12(1+cos⁡2θ)\cos^2\theta = \tfrac12(1 + \cos 2\theta), the cos⁡2θ\cos 2\theta term averages to zero over a full turn, leaving the mean equal to 12\tfrac12. Hence the first filter transmits I0/2I_0/2, equation (1) — no matter which way its axis points.

Step 4. Chain them. Unpolarized I0I_0 → first filter → I0/2I_0/2, polarized along axis 1 → analyser at θ\theta → (I0/2)cos⁡2θ(I_0/2)\cos^2\theta, equation (3). At θ=45∘\theta = 45^\circ that is (I0/2)(0.5)=I0/4(I_0/2)(0.5) = I_0/4; at θ=90∘\theta = 90^\circ it is zero. Verified: the average of cos⁡2\cos^2 over a full turn equals 1/21/2, and cos⁡2θ\cos^2\theta at 0∘,30∘,45∘,60∘,90∘0^\circ, 30^\circ, 45^\circ, 60^\circ, 90^\circ equals 1,0.75,0.5,0.25,01, 0.75, 0.5, 0.25, 0 — recomputed in verify_hs2-polarization.py.

The crossed-filters trick: three do what two cannot

Cross two filters (θ=90∘\theta = 90^\circ) and nothing gets through — Malus's law gives cos⁡290∘=0\cos^2 90^\circ = 0. Now insert a third filter between them, at 45∘45^\circ to both. Astonishingly, light reappears. Track it with Malus's law twice. Unpolarized light IuI_u enters and the first filter gives Iu/2I_u/2, polarized vertically. The middle filter at 45∘45^\circ transmits (Iu/2)cos⁡245∘=Iu/4(I_u/2)\cos^2 45^\circ = I_u/4, and re-polarizes the light to 45∘45^\circ. The last filter, at 90∘90^\circ to the first but only 45∘45^\circ from the middle one, transmits (Iu/4)cos⁡245∘=Iu/8(I_u/4)\cos^2 45^\circ = I_u/8:

I=Iu2cos⁡245∘cos⁡245∘=Iu2⋅12⋅12=Iu8=0.125 Iu.(4)I = \frac{I_u}{2}\cos^2 45^\circ \cos^2 45^\circ = \frac{I_u}{2}\cdot\frac12\cdot\frac12 = \frac{I_u}{8} = 0.125\,I_u. \qquad (4)

The middle filter rotates the polarization in two 45∘45^\circ steps, so the crossed pair no longer sees a right angle across a single gap. Remove the middle filter and you are back to cos⁡290∘=0\cos^2 90^\circ = 0. This is the famous demonstration that a polarizing filter does not merely "select" light already present — it re-projects the field, and inserting an element can increase what passes downstream.

Limiting cases

caseresultmeaning
unpolarized into 1 filterI=I0/2I = I_0/2half survives, whatever the axis direction
axes aligned, θ=0\theta = 0I=I1I = I_1analyser fully open, Malus gives cos⁡20=1\cos^2 0 = 1
axes at 45∘45^\circI=I1/2I = I_1/2half through; cos⁡245∘=0.5\cos^2 45^\circ = 0.5
axes crossed, θ=90∘\theta = 90^\circI=0I = 0dark; cos⁡290∘=0\cos^2 90^\circ = 0
third filter at 45∘45^\circ between crossed pairI=Iu/8I = I_u/8light reappears — the middle filter rotates the polarization
longitudinal wave (sound)no effectcannot be polarized — no transverse direction to block

Worked examples

Board level — two filters at an angle (CBSE and NEET pattern)

Unpolarized light of intensity I0I_0 passes through two polarizing filters whose transmission axes are at 30∘30^\circ to each other. (a) What fraction emerges? (b) What if the angle is 60∘60^\circ?

Step 1. First filter halves the unpolarized light: I1=I0/2I_1 = I_0/2, polarized along axis 1.

Step 2. Second filter, Malus's law at θ=30∘\theta = 30^\circ: I=I1cos⁡230∘=(I0/2)(0.75)=0.375 I0I = I_1\cos^2 30^\circ = (I_0/2)(0.75) = \boxed{0.375\,I_0}, i.e. three-eighths.

Step 3. For θ=60∘\theta = 60^\circ: I=(I0/2)cos⁡260∘=(I0/2)(0.25)=0.125 I0I = (I_0/2)\cos^2 60^\circ = (I_0/2)(0.25) = \boxed{0.125\,I_0}, i.e. one-eighth.

Step 4. Sense-check: increasing the angle from 30∘30^\circ to 60∘60^\circ cut the output from 0.375 I00.375\,I_0 to 0.125 I00.125\,I_0 — dimmer, as it must, since the axes are further from aligned. At 90∘90^\circ it would be zero.

Board level — reading off the angle (ICSE and JEE pattern)

Polarized light of intensity I1I_1 falls on an analyser. At what angle is the transmitted intensity (a) half of I1I_1, and (b) one-quarter of I1I_1?

Step 1. Half: set cos⁡2θ=0.5\cos^2\theta = 0.5, so cos⁡θ=1/2\cos\theta = 1/\sqrt2 and θ=45∘\theta = \boxed{45^\circ}.

Step 2. One-quarter: set cos⁡2θ=0.25\cos^2\theta = 0.25, so cos⁡θ=0.5\cos\theta = 0.5 and θ=60∘\theta = \boxed{60^\circ}.

Step 3. Note the pattern for later recall: 30∘→0.7530^\circ \to 0.75, 45∘→0.545^\circ \to 0.5, 60∘→0.2560^\circ \to 0.25 — the outputs step down as the angle climbs, symmetric about 45∘45^\circ being the half-power point.

Step 4. Caution: these angles are between the analyser and the already-polarized beam. If the source were unpolarized, the first filter would separately contribute its own factor of 12\tfrac12.

Competitive level — the three-filter surprise (JEE-Advanced and NEET pattern)

Two polarizing filters are crossed (90∘90^\circ apart) so no light passes. Unpolarized light of intensity IuI_u is incident. A third filter is now inserted between them at 45∘45^\circ to each. (a) What intensity emerges? (b) What emerges if the third filter is instead placed at 30∘30^\circ to the first?

Step 1. First filter: Iu/2I_u/2, polarized vertically. Middle filter at 45∘45^\circ: (Iu/2)cos⁡245∘=Iu/4(I_u/2)\cos^2 45^\circ = I_u/4, now polarized at 45∘45^\circ. Last filter (at 90∘90^\circ from first, so 45∘45^\circ from middle): (Iu/4)cos⁡245∘=Iu/8=0.125 Iu(I_u/4)\cos^2 45^\circ = \boxed{I_u/8 = 0.125\,I_u}.

Step 2. Part (b): middle filter at 30∘30^\circ from the first, so 60∘60^\circ from the last. After first: Iu/2I_u/2. After middle: (Iu/2)cos⁡230∘=(Iu/2)(0.75)=0.375 Iu(I_u/2)\cos^2 30^\circ = (I_u/2)(0.75) = 0.375\,I_u. After last: (0.375 Iu)cos⁡260∘=(0.375 Iu)(0.25)=0.09375 Iu(0.375\,I_u)\cos^2 60^\circ = (0.375\,I_u)(0.25) = \boxed{0.09375\,I_u}.

Step 3. The maximum output over all middle-filter angles is at 45∘45^\circ, giving Iu/8I_u/8 — you can see this because the transmitted fraction 12cos⁡2θcos⁡2(90∘−θ)=12cos⁡2θsin⁡2θ\tfrac12\cos^2\theta\cos^2(90^\circ-\theta) = \tfrac12\cos^2\theta\sin^2\theta peaks where cos⁡θ=sin⁡θ\cos\theta = \sin\theta, i.e. θ=45∘\theta = 45^\circ.

Step 4. The headline: crossed filters that pass nothing can be made to pass one-eighth of the incident light by inserting a filter between them. Removing that middle filter drops the output straight back to zero. Timing note: about 90 seconds. The whole problem is "12\tfrac12 for the first filter, then cos⁡2\cos^2 of each successive angle." Do not forget the initial 12\tfrac12, and always measure each angle from the light's current polarization, not from a fixed axis.

Exam traps

Using cos⁡2θ\cos^2\theta at the first filter. Unpolarized light halves — I0/2I_0/2 — regardless of the filter's orientation, because it carries all polarization directions equally and the average of cos⁡2\cos^2 is 12\tfrac12. Only after the light is polarized does a definite θ\theta exist for Malus's law. This single confusion sinks more marks than any other in the topic.

Thinking crossed filters can never pass light. Two crossed filters pass zero, but a third filter placed between them at any angle other than 0∘0^\circ or 90∘90^\circ lets light through — Iu/8I_u/8 at the optimal 45∘45^\circ. The middle filter re-projects (rotates) the polarization, so the outer pair is no longer crossed across a single step.

Measuring the analyser angle from the wrong reference. In a multi-filter stack, the θ\theta in each Malus factor is the angle between the light's current polarization direction (set by the previous filter) and the next axis — not the angle to the original first filter. Chain the angles filter by filter.

Claiming sound or any longitudinal wave can be polarized. It cannot: a longitudinal oscillation is along the travel direction and has no transverse "sideways" to block. Polarization is precisely the experiment that distinguishes transverse light from longitudinal sound.

Board scope. Polarization and Malus's law are examined by CBSE, ICSE, JEE-Main, JEE-Advanced and NEET. They are a structural zero on IB (both SL and HL) and on A-Level 9702 — those syllabuses do not cover polarization at all, so do not spend IB or CIE revision on it. The current AP Physics 2 (Fall-2024 Unit 14) also omits polarization from its topic list. This is an India-facing topic; if your board is IB, A-Level or AP, you can safely skip it.

Origins · 1 minÉtienne-Louis Malus and how this was discovered
ÉM
Étienne-Louis Malus
1775–1812 · Paris

Étienne-Louis Malus was a French army engineer who followed Napoleon to Egypt and returned to make one of optics' great chance discoveries. One evening in 1808, looking through a crystal of Iceland spar at sunlight reflected from the windows of the Luxembourg Palace, he noticed the reflected light brightened and dimmed as he rotated the crystal — reflection had done to the light what a crystal does. He had found that light could be polarized by reflection, and he coined the very word "polarization." Pressing on, he measured how the transmitted intensity varied with angle and, in 1809, published the law that bears his name, I=I0cos⁡2θI = I_0\cos^2\theta — the first quantitative law of polarization and a cornerstone of modern wave optics. The Académie des Sciences awarded him its prize in 1810 for his theory of double refraction, the same body of work, and he died young, at 36, of an illness likely contracted on the Egyptian campaign.

History
1669
— Erasmus Bartholin describes double refraction in Iceland spar, the first recorded polarization effect, without explaining it.
1808
— Étienne-Louis Malus discovers polarization by reflection off the Luxembourg Palace windows and coins the term polarization.
1809
— Malus publishes his law, I = I₀cos²θ, the first quantitative description of polarized light.
1815
— David Brewster finds the angle at which reflected light is completely polarized, linking polarization to the refractive index.
1852
— William Bird Herapath discovers herapathite, the light-polarizing crystal later used to make sheet Polaroid filters.

Going further

Texts. NCERT Physics Class 12, Ch. 10 ("Wave Optics"), §10.7 on polarization and Malus's law · H. C. Verma, Concepts of Physics Vol. 1, "Light Waves," polarization section · Halliday, Resnick and Walker, "Polarization," for the field-projection picture.

Provenance. Standard results. Recompute: first-filter transmission I0/2I_0/2 (average of cos⁡2\cos^2 over a full turn =0.5= 0.5); Malus cos⁡2θ\cos^2\theta at 0∘,30∘,45∘,60∘,90∘=1,0.75,0.5,0.25,00^\circ, 30^\circ, 45^\circ, 60^\circ, 90^\circ = 1, 0.75, 0.5, 0.25, 0; two filters at 30∘30^\circ: 0.375 I00.375\,I_0; at 60∘60^\circ: 0.125 I00.125\,I_0; crossed pair with 45∘45^\circ middle: Iu/8=0.125 IuI_u/8 = 0.125\,I_u; crossed pair with 30∘30^\circ middle: 0.09375 Iu0.09375\,I_u; half-intensity angle 45∘45^\circ; quarter-intensity angle 60∘60^\circ; three-filter maximum at 45∘45^\circ.

Prerequisites. The Nature of Electromagnetic Waves — where the transverse electric field this article confines comes from. Leads to. Brewster's Law and Polarization by Reflection/Scattering — polarization "for free," no filter needed · the university seams Polarization of Light and Malus's Law.

Go deeper (UG). The full Stokes-parameter description of polarization states — linear, circular, elliptical, and partially polarized light — is developed in Polarization of Light, and the field-projection argument is generalised in Malus's Law. Enrichment only; nothing above is needed to follow this article.

Why does unpolarized light lose exactly half, not some other fraction?

Because unpolarized light contains every transverse polarization direction with equal weight, and each direction is reduced by cos⁡2θ\cos^2\theta as it meets the filter's axis. Averaging cos⁡2θ\cos^2\theta over a full circle of directions gives exactly one half — the cos⁡2\cos^2 curve spends as much "area" above the value 12\tfrac12 as below it. So the first filter always transmits I0/2I_0/2, and turning the filter changes only which direction survives, not how much. The one-half is a property of the random input, not of any particular angle, which is why you must not plug an angle into Malus's law for the first filter.

Is Malus's law about the electric field or the intensity?

Both, in sequence. The filter acts on the electric field: it passes the component Ecos⁡θE\cos\theta along its axis. But what your eye or a detector measures is intensity, which is proportional to the field squared. Squaring Ecos⁡θE\cos\theta turns the field's single power of cos⁡θ\cos\theta into the intensity's cos⁡2θ\cos^2\theta. That is the whole content of Malus's law: project the field (one cos⁡θ\cos\theta), then square for intensity (giving cos⁡2θ\cos^2\theta). Getting this order right also explains why the maximum is a broad, flat peak near θ=0\theta = 0, the intensity falls fastest around θ=45∘\theta = 45^\circ, then flattens again as it approaches zero near 90∘90^\circ.

Can you really get light through two filters that separately block it?

The two crossed filters do not each "block" the light — the first one polarizes it (passing half), and the second, being crossed, then passes none of that polarized beam. Insert a third filter at 45∘45^\circ between them and it rotates the polarization halfway, so the final filter is only 45∘45^\circ from the light reaching it and passes half again. The net is Iu/8I_u/8. Nothing is created from nothing: you started with IuI_u, the first filter already discarded half, and the middle filter's job is to rotate what remains so the last filter no longer sees a right angle. It is one of the most memorable demonstrations in optics precisely because it defies the naive "crossed means dark, always" intuition.

Why can't sound be polarized?

Sound is a longitudinal wave: the air oscillates back and forth along the direction the wave travels, compressing and rarefying. There is no sideways oscillation to confine, so there is nothing for a "sound polarizer" to select — the concept does not apply. Light is different: its electric field oscillates across the travel direction, so it has a transverse orientation that a filter can pick out. This is exactly why polarization was such decisive evidence. Interference and diffraction happen for both transverse and longitudinal waves and so cannot tell them apart, but only a transverse wave can be polarized — so the fact that light polarizes proves it shakes sideways.

Do polarizing sunglasses work by Malus's law?

Yes, with a twist about the source. Glare reflected off a horizontal surface like water or a road is already partially polarized in the horizontal direction (that is the Brewster effect of the next article). Polarizing sunglasses fix their transmission axis vertical, so for the horizontally polarized glare the angle is near 90∘90^\circ and cos⁡2θ\cos^2\theta is small — the glare is cut. For the rest of the scene, which is roughly unpolarized, the lenses simply pass about half, dimming everything a little. That is why tilting your head sideways while wearing them makes glare flare back: you have rotated your axis toward the glare's polarization, raising cos⁡2θ\cos^2\theta.

If my board is IB or A-Level, do I need this at all?

No. Polarization and Malus's law are not on IB (SL or HL) or on A-Level 9702 — those specifications simply do not include the topic, and the current AP Physics 2 Unit 14 also omits it. This is India-facing content, examined by CBSE, ICSE, JEE-Main, JEE-Advanced and NEET. If you are sitting one of those, learn it thoroughly — the I0/2I_0/2-then-cos⁡2θ\cos^2\theta chain and the three-filter trick are reliable exam earners. If you are an IB, A-Level or AP student, you can read this for interest but spend your revision time on the interference and diffraction topics your board actually assesses.

Before this

Where this leads