INGENIA

WAV-07

Malus's law

I = I0 cos² θ after an ideal polariser.

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PolarisationMalus 1808

Governing equation

I=I0cos⁡2θI=I_0\cos^2\theta

θ∈[0,90]\theta \in \left[0, 90\right]

where

I_0
Incident intensity (W/m²)
\theta
Angle to axis (°)
I
Transmitted intensity (W/m²)

The figure, part by part

Each numbered marker wears the color of its card. Hover a card to light the marker. Tap a marker to jump to that card. The slider walks a red point along the curve; Animate drawing traces it like a pen.

WAV-07 · lens
00:0 / 00:08
①

Governing law — red

I=I0cos⁡2θI=I_0\cos^2\theta

θ∈[0,90]\theta \in \left[0, 90\right]

θ=0\theta = 0I=1I = 1

②

Domain of the variable — blue

θmin⁡=0,θmax⁡=90\theta_{\min} = 0,\quad \theta_{\max} = 90

θ∈[0,90]\theta \in \left[0, 90\right]

θ=0\theta = 0θ=0\theta = 0

③

Response curve — green

I=I0cos⁡2θI=I_0\cos^2\theta

θ∈[0,90]\theta \in \left[0, 90\right]

θ=0\theta = 0I=1I = 1

④

Rate of change — amber

dIdθ\frac{\mathrm{d}I}{\mathrm{d}\theta}

θ∈[0,90]\theta \in \left[0, 90\right]

θ=0.566\theta = 0.566I′=−3.45×10−4I^{\prime} = -3.45\times 10^{-4}

Lecture brief

Historical brief

d’Alembert’s wave equation, Snell, the thin-lens maker, Doppler and Bragg interference are the classical optics-and-sound toolkit. The lab is propagation, image and shift. This sheet (WAV-07 — Malus's law) is the form associated with Malus 1808. Working symbols: I0I_0, θ\theta →\rightarrow II. The transmitted amplitude is the projection of E onto the polariser axis, so intensity — the square — follows cos² θ.

Purpose

Purpose: compute II from I0I_0, θ\theta in Waves & optics via I=I0cos⁡2θI=I_0\cos^2\theta I = I0 cos² θ after an ideal polariser. Use it when a real waves & optics question must be answered in SI before a code check.

Live realistic example

In symbols

Live case. Given I0=1.000 W/m2I_0 = 1.000\,\mathrm{W/m^{2}}, θ=35.000 ∘\theta = 35.000\,\mathrm{^{\circ}}, the governing relation I=I0cos⁡2θI=I_0\cos^2\theta yields I=0.6710 W/m2I = 0.6710\,\mathrm{W/m^{2}}. Linearly polarised input, lossless polariser. Move a slider: the numbers are this situation, not a canned story.

Calculator

Inputs

Outputs

  • Transmitted intensity I0.6710 W/m²
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WAV-07 · lens
00:0 / 00:08

Narration of this film

Linearly polarised input, lossless polariser.

The transmitted amplitude is the projection of E onto the polariser axis, so intensity — the square — follows cos² θ.

Reading speed

Watch on YouTube