How Do Ψ and Δ Reveal Thin-Film Changes? An Introduction to Ellipsometry

Observe SiO2 thickness changes with the ellipsometric parameters Ψ and Δ

The reflectance change from a transparent film can be small even when the polarization of the reflected light has changed substantially. Ellipsometry uses that change: Ψ and Δ jointly measure the amplitude ratio and phase difference between p- and s-polarized reflection.

This tutorial builds a first ellipsometry model for an air / SiO₂ / Si structure, then sweeps the SiO₂ thickness from 50 to 150 nm. By the end, you can configure an ellipsometry calculation, read Ψ/Δ spectra, and identify spectral regions that are more sensitive to film thickness.

Laboratory ellipsometer with source and detector arms on either side of the sample stage
An ellipsometer measures how oblique reflection changes the polarization stateGuillaume Paumier / Wikimedia CommonsCC BY-SA 3.0

What Ψ and Δ Mean

Incident light can be resolved into p polarization parallel to the plane of incidence and s polarization perpendicular to it. Let rpr_p and rsr_s be their complex amplitude reflection coefficients. The ellipsometric ratio is

ρ=rprs=tanΨexp(iΔ).\rho=\frac{r_p}{r_s}=\tan\Psi\,\exp(\mathrm{i}\Delta).

Here, ρ\rho is the complex ellipsometric ratio; rpr_p and rsr_s are the complex amplitude reflection coefficients for p and s polarization; Ψ\Psi describes their amplitude ratio; Δ\Delta describes their phase difference; and i\mathrm{i} is the imaginary unit. Ψ and Δ must be used together to describe the change in the polarization ellipse completely.

Ellipsometry setup with light source polarizer sample compensator analyzer and detector
A typical ellipsometry path: known polarized light reflects from the sample and enters polarization analysis and detectionBuntgarn, Stannered / Wikimedia CommonsCC BY-SA 3.0

Ellipsometry is normally performed at oblique incidence, where the p and s reflection responses differ more strongly. A change in film thickness or refractive index changes the optical phase thickness, shifting or reshaping the Ψ and Δ spectra.

Build the SiO₂ / Si Model

Create an air / SiO₂ / Si structure. Use wavelength-dependent optical constants for a 100 nm SiO₂ film. Treat silicon as the semi-infinite bottom medium rather than adding a millimeter-scale coherent film.

PositionMaterialSetting
Top mediumAirn=1.00n=1.00, k=0k=0
FilmSiO₂100 nm, wavelength-dependent index
Bottom mediumSiWavelength-dependent complex index
Structure settings for a 100 nm SiO2 film on a silicon bottom medium in air
Figure 1 | 100 nm SiO₂ / Si ellipsometry model

Configure Oblique-Incidence Ellipsometry

On the Optics page, use 400–800 nm with a 2 nm step and an incidence angle of 70°. Enable Psi and Delta. The ellipsometric parameters are calculated from the ratio of p and s reflection coefficients; pRatio is not an experimental polarizer angle that needs to be swept.

Optical settings from 400 to 800 nm at 70 degrees with Psi and Delta enabled
Figure 2 | Wavelength, angle, and detector settings for ellipsometry

Read Ψ and Δ for the 100 nm Film

Run the calculation and open Psi first.

Psi ellipsometry spectrum of a 100 nm SiO2 film on silicon
Figure 3 | Ψ spectrum of 100 nm SiO₂ / Si

Ψ describes the changing ratio of p and s reflection amplitudes. At 550 nm, Ψ is about 0.906 rad (51.90°) for the 100 nm film. The spectral shape combines thin-film interference with the complex refractive index of silicon.

Delta ellipsometry spectrum of a 100 nm SiO2 film on silicon
Figure 4 | Δ spectrum of 100 nm SiO₂ / Si

Δ is the phase difference between p and s reflection. At 550 nm, it is about 1.653 rad (94.70°). The result page displays phase in a principal range. When a curve crosses the boundary it may jump from a positive to a negative value; this is phase wrapping, not a physical discontinuity in the sample response.

Sweep Thickness and Watch the Spectra Move

On the Sweep page, add SiO2 Film → Thickness from 50 to 150 nm with a 25 nm step.

Parameter sweep of SiO2 thickness from 50 to 150 nm in 25 nm steps
Figure 5 | SiO₂ thickness Sweep
Psi ellipsometry spectra for five SiO2 film thicknesses
Figure 6 | Ψ spectra as SiO₂ thickness changes

As thickness increases from 50 to 150 nm, the Ψ maximum moves progressively toward longer wavelengths. The curves do not simply shift vertically: both peak position and line shape change, so a full spectrum contains more thickness information than one wavelength.

Delta ellipsometry spectra for five SiO2 film thicknesses
Figure 7 | Δ spectra as SiO₂ thickness changes

Δ is also sensitive to thickness, and the location of phase wrapping moves with the film. When comparing or fitting curves, use a consistent phase representation rather than interpreting jumps between 2π2\pi-equivalent values as large errors.

At 550 nm, the results are:

SiO₂ thicknessΨΔ
50 nm25.98°87.17°
75 nm35.37°98.02°
100 nm51.90°94.70°
125 nm83.94°−42.83°
150 nm48.22°−96.36°

The negative Δ values for 125 and 150 nm follow from the selected principal range. Their equivalent unwrapped values are 317.17° and 263.64°.

From a Forward Model to Thickness Measurement

This Sweep establishes the basic ellipsometric distinction: different film thicknesses produce distinguishable Ψ/Δ spectra. In a measurement workflow, experimental curves are compared with a model containing material optical constants, surface layers, and thickness variables, and the joint residual of Ψ and Δ is used to judge the parameters.

Using Ψ alone discards phase information; using Δ alone can leave phase-wrapping ambiguities. Use both curves and prefer spectral regions that are sensitive to the target parameter and supported by reliable material data. This tutorial performs forward sensitivity analysis, not automatic inversion of measured data.

Variation Exercise

Keep SiO₂ at 100 nm and sweep incidence angle from 60° to 75° in 5° steps. Compare Ψ and Δ near 550 nm and decide whether 70° distinguishes 75 nm from 100 nm more clearly than 60°.


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