Polynomial-exponent modeling and identification of the white-light scanning interferogram
Summary
This study introduces a new polynomial-exponent model and algorithm for analyzing white-light interferograms. It accurately determines fringe phase and dispersion, crucial for precise optical measurements.
Area of Science:
- Optics and Photonics
- Metrology
- Signal Processing
Background:
- White-light interferometry is vital for precise measurements but analyzing complex interferograms is challenging.
- Existing models may not fully capture variations in fringe and envelope patterns caused by light sources or dispersive media.
Purpose of the Study:
- To develop a robust polynomial-exponent model for white-light interferograms.
- To introduce a direct fast Fourier transform (FFT)-based algorithm for accurate interferogram analysis.
- To enable precise estimation of phase and dispersion parameters.
Main Methods:
- A polynomial-exponent model is formulated, incorporating differential equations and frequency-domain analysis.
- A two-step algorithm is proposed: 1) polynomial coefficient estimation, 2) amplitude and phase estimation.
- A method for calculating the dispersion parameter as a quadratic phase component is developed.
Main Results:
- The model accurately describes diverse envelope and fringe phase distributions.
- The algorithm successfully estimates fringe phase, even when unknown, at the envelope peak.
- Dispersion parameters are calculated with high accuracy, approaching the Cramér-Rao lower bound.
Conclusions:
- The proposed model and FFT-based algorithm offer a precise and efficient method for white-light interferogram analysis.
- This approach enhances the accuracy of optical metrology, particularly in the presence of dispersive effects.
- The technique provides a reliable framework for extracting higher-order interferogram parameters.


