Model films using thickness, wavelength, and index. Add absorption or angle settings for deeper accuracy. Get clear outputs that support faster optical design decisions.
| n0 | n | t (nm) | λ (nm) | θ0 (deg) | Optical thickness n·t (nm) | Phase δ (deg) |
|---|---|---|---|---|---|---|
| 1.000 | 1.500 | 500 | 550 | 0 | 750 | 490.9 |
| 1.000 | 2.100 | 110 | 532 | 0 | 231 | 156.2 |
| 1.000 | 1.450 | 95 | 633 | 30 | 137.8 | 74.9 |
Physical thickness t is a geometric length. Optical thickness n*t scales that length by refractive index and indicates how strongly the film can affect propagation. A 100 nm layer at n = 2.0 has the same n*t as a 200 nm layer at n = 1.0. Use this result when comparing materials with different indices.
Interference in thin films depends on the phase thickness delta = (2*pi/lambda)*n*t*cos(theta_t). When delta changes by 2*pi, reflected and transmitted behavior repeats. Values near pi/2 correspond to quarter-wave designs, while pi corresponds to half-wave. The calculator reports delta in radians and degrees for quick checks.
At oblique incidence, phase depends on cos(theta_t), where theta_t is the internal angle inside the film. The tool computes theta_t from n0*sin(theta0) = n*sin(theta_t). If n0 is larger than n and theta0 is large, total internal reflection conditions can occur, and the page flags this for caution.
For a chosen wavelength, quarter-wave thickness tQW = lambda/(4*n*cos(theta_t)) sets delta = pi/2 and is widely used for anti-reflection stacks. Half-wave thickness tHW = lambda/(2*n*cos(theta_t)) sets delta = pi and is useful for spacers or phase correction. Compare your t to these targets to gauge design intent.
Coatings are usually specified at application wavelengths. Pick a wavelength that matches your source, such as 532 nm, 633 nm, or 1550 nm. If you work across a band, run several wavelengths to see how delta and the quarter-wave target shift. Thickness stays fixed, but phase scales inversely with lambda.
Real films can absorb. If you know absorption coefficient alpha in 1/m, optical depth is tau = alpha*t. If you instead know extinction coefficient k, the calculator derives alpha = 4*pi*k/lambda and then tau. A baseline absorption-only transmission estimate is T = exp(-tau), which ignores reflections and interference.
Optical thickness is central in ellipsometry models and in fringe behavior in transmission spectra. Small changes in n or t can shift delta enough to move a minimum or maximum. By adjusting n, t, and lambda, you can run sensitivity checks, estimate phase error from tolerances, and keep unit-consistent values for documentation.
Refractive index can be dispersive and complex, so use values appropriate to your wavelength and process. Keep angles below 90 degrees and confirm which medium defines theta0. When exporting CSV or PDF, record the same units used in setup. For full coating performance, combine these outputs with matrix-based thin-film models.
It is the optical path contribution of the layer, defined as n*t. It helps compare films made of different materials and indicates how strongly the layer can influence phase.
Phase accumulation depends on the component of propagation normal to the interfaces. Inside the film, that projection introduces cos(theta_t), where theta_t is the internal angle found from Snell's relation.
Yes, if you use a nonzero incidence angle. n0 affects theta_t through Snell's relation. For normal incidence, n0 has no impact on phase thickness.
It is best for single-layer checks and targets like quarter-wave and half-wave thickness. For multilayer stacks, you still can compute each layer's phase thickness, but full reflectance needs matrix calculations.
Enter k and the wavelength. The calculator converts it to alpha using alpha = 4*pi*k/lambda, then computes optical depth tau and a basic transmission estimate.
The exp(-tau) result models absorption only. Real transmission also includes Fresnel reflections, interference fringes, scattering, and substrate effects. Use it as a baseline when absorption is the dominant loss.
Nanometers are convenient for thin films and visible wavelengths, while micrometers are common in infrared. Any supported unit works, because the calculator converts internally to meters before computing results.
Important Note: All the Calculators listed in this site are for educational purpose only and we do not guarentee the accuracy of results. Please do consult with other sources as well.