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Radiometric errors in complex Fourier transform spectrometry.
1Space Science and Engineering Center, University of Wisconsin, Madison, 1225 West Dayton Street, Madison, Wisconsin 53706, USA. larry.sromovsky@ssec.wisc.edu
Applied Optics
|April 10, 2003
Summary
This study derives the root-mean-square noise in the real part of a complex spectrum, confirming the commonly used noise relation. It also presents a variance equation for real spectra derived from complex calibration, accounting for reference spectrum uncertainties.
Area of Science:
- Spectroscopy
- Optical Engineering
- Signal Processing
Background:
- Fourier transforms of asymmetric interferograms produce complex spectra.
- Understanding spectral noise is crucial for accurate measurements.
- Existing noise relations require rigorous validation in complex spectral analysis.
Purpose of the Study:
- To rigorously derive and validate the root-mean-square (rms) noise in the real part of a complex spectrum.
- To establish a variance equation for real spectra obtained through complex calibration.
- To quantify the impact of uncertainties in reference spectra on the final spectral variance.
Main Methods:
- Fourier transform analysis of asymmetric interferograms.
- Rigorous mathematical derivation of noise and variance equations.
- Complex calibration techniques using hot and cold reference spectra.
Main Results:
- Confirmed the commonly used relation for rms noise in the real part of the spectrum: sigmaR = 2X x NEP/(etaAomega square root(tauN)).
- Derived a new variance equation for real spectra: sigmaL2 = sigmaR2 + sigma(c)2 (Lh - Ls)2/(Lh - Lc)2 + sigma(h)2 (Ls - Lc)2/(Lh - Lc)2.
- The derived equations are valid under conditions where spectral noise and uncertainties are small relative to spectral differences.
Conclusions:
- The study provides a rigorous theoretical foundation for noise analysis in complex spectral data.
- The findings are essential for improving the accuracy and reliability of spectroscopic measurements, particularly in applications involving asymmetric interferograms.
- Accurate characterization of noise and reference spectra uncertainties is critical for precise spectral analysis.