Spectroscopic ellipsometry is a non-destructive, noncontact, and non-invasive optical technique which is based on the change in the polarization state of light as it is reflected obliquely from a thin film sample. Ellipsometry uses a model based approach to determine thin film, interface, and surface roughness thicknesses, as well as optical properties (and much more!) for thin films ranging in thickness from a few A to several tens of microns.
Also, spectroscopic ellipsometry can be performed either ex-situ or in-situ, in static or kinetic mode, for various application needs.
Spectroscopic ellipsometry measures ψ and Δ, both of which describe the output elliptical polarization state after linearly polarized light is reflected obliquely off of a thin film sample.
The parameters ψ and Δ are related to the complex Fresnel reflection coefficients according to: ρ = tan ψ eiΔ = rp / rs. After collecting ψ and Δ, a model representing the thin film structure must be built in order to determine thickness and/or optical constants
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