Paritian

Physics

Malus's Law Calculator (Polarisers)

Light intensity after one, two or three polarisers at any angles, with the classic three-polariser surprise shown on the chart.

Results

After the first polariser 50 W/m²
After the second polariser 25 W/m²
After the third polariser 12.5 W/m²
After the third, without the middle one 1.8747e-31 W/m²
Share of the light that gets through 12.50 %
How it changes
Light through the polarisersAngle of the second polariser 0 – 180. After the second polariser: 50 → 50; After the third polariser: 1.8747e-31 → 1.8747e-31; After the third, without the middle one: 1.8747e-31 → 1.8747e-31After the second polariserAfter the third polariserAfter the third, without the middle one01020304050050100150Angle of the second polariser (°)

The dashed line marks the value you entered.

What this tool does

Malus's law says a polariser passes the fraction cos²θ of light that is already polarised, θ being the angle between the light's polarisation and the polariser's axis; unpolarised light loses half at the first filter whatever its angle. The famous surprise comes with three: two crossed polarisers block everything, yet a third slipped between them at 45° lets an eighth of the original light through. Angles are measured from the first polariser. Real polarisers absorb a little even when aligned, so measured values come out somewhat lower.

Formula

I = I₀ cos² θ · unpolarised light through one polariser: I = I₀ ÷ 2

Variables

SymbolMeaningUnit
i0Incoming light intensityW/m²
upLight reaching the first polariser—
a1Angle of the second polariser°
a3Angle of the third polariser°
I1After the first polariserW/m²
I2After the second polariserW/m²
I3After the third polariserW/m²
IXAfter the third, without the middle oneW/m²
TRShare of the light that gets through%

Worked example

  • Incoming light intensity100 W/m²
  • Light reaching the first polariser1
  • Angle of the second polariser45 °
  • Angle of the third polariser90 °
  • After the first polariser50 W/m²
  • After the second polariser25 W/m²
  • After the third polariser12.5 W/m²
  • After the third, without the middle one1.8747e-31 W/m²
  • Share of the light that gets through12.50 %

Limitations

  • The formula assumes ideal conditions: no friction losses, no air resistance and no efficiency losses unless you enter them.
  • Mixing units is the most common source of error. Convert every input to the units shown next to each field before calculating.