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Uncertainty Propagation for NIST Visible Spectral Standards
1CSIRO National Measurement Laboratory Lindfield, Australia 2070.
Summary
This study details how uncertainties in National Institute of Standards and Technology (NIST) spectral standards are calculated. It provides a framework for accurate radiometric measurements by accounting for correlations in spectral data.
Area of Science:
- Metrology
- Optical Engineering
- Radiometry
Background:
- Accurate spectral standards are crucial for reliable detector and source characterization.
- Existing methods for uncertainty propagation in spectral measurements require refinement, especially considering wavelength correlations.
Purpose of the Study:
- To propagate uncertainties in NIST spectral standards for detectors and sources in the visible range.
- To detail uncertainty propagation through fitting and transfer spectral measurements.
- To provide recommendations for interpolating spectral irradiance values.
Main Methods:
- High accuracy cryogenic radiometer measurements were used as the basis for uncertainty propagation.
- Partial correlations between spectral values at different wavelengths were estimated.
- Uncertainty propagation was analyzed through fitting, transfer spectral measurements, and the spectral comparator facility.
Main Results:
- A comprehensive method for propagating uncertainties in spectral standards, considering correlations, was developed.
- Detector uncertainties were successfully propagated for external calibrations and internal photometric quantities.
- Uncertainties in spectral irradiance were derived and propagated to calibrated artifacts.
Conclusions:
- The developed method provides a robust framework for assessing uncertainties in spectral standards.
- Accurate estimation of correlations is vital for precise radiometric calculations.
- Interpolation is recommended over fitting for NIST-provided spectral irradiance values to minimize uncertainty.

