Polarimetry Bench

2D view of the 3D polarimetry controller: a rotating analyzer samples the light, and a fit recovers its polarization state.

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Model checks

The science

What is modelled

Fully polarized monochromatic light is described by a Stokes vector (S0, S1, S2, S3). An optical rotator turns the linear axis, a linear retarder delays one component and can make the light elliptical, and an ideal analyzer passes the component along its axis.

Equations

  • Linear input S = (1, cos 2ψ, sin 2ψ, 0).
  • Analyzer I = ½ (S0 + S1 cos 2α + S2 sin 2α), which reduces to Malus's law cos2(α - ψ) for linear light.
  • Retarder: rotate Q/U into the fast-axis frame, then rotate U/V by the retardance.
  • Scan fit I = A + B cos 2α + C sin 2α by linear least squares.

Checks run in the page

  • Malus's law across many angles.
  • The total degree of polarization stays 1 through lossless optics.
  • The scan fit recovers the linear polarization fraction.
  • Quarter- and half-wave plate behaviour.

Honest simplifications

Ideal monochromatic and fully polarized light, ideal wave plates and a leakage term for the analyzer; no depolarization or wavelength dependence.

What to try
  • Choose Quarter-wave to circular: the analyzer scan becomes flat because circular light passes every angle equally.
  • Choose Pure linear and compare the curve with cos squared.
  • Raise the detector noise and see how the fit residual grows while the fitted angle stays close.
Intensity against analyzer angle
Stokes parameters against retardance
Linear and circular polarization fractions
Fit residuals
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