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Technique for measuring the reflectance of irregular, submillimeter-sized samples
Applied Optics
|September 11, 2010
Summary
This study presents a novel technique for measuring the reflectance of small, irregular samples across a wide spectral range (far IR to visible) and temperature range (10–300 K). The method corrects for scattering and diffraction, providing accurate specular reflectance measurements.
Area of Science:
- Spectroscopy
- Optical Physics
- Materials Science
Background:
- Accurate optical characterization of small, irregular samples is crucial for understanding material properties.
- Existing techniques often struggle with sample size limitations and complex scattering effects.
Purpose of the Study:
- To develop and validate a versatile technique for measuring the near-normal incidence reflectance of submillimeter-sized, irregular samples.
- To cover a broad spectral range from the far-infrared to the visible spectrum.
- To enable measurements at cryogenic temperatures (10–300 K).
Main Methods:
- Utilized a modified Michelson interferometer or grating spectrometer.
- Employed nonreflecting cones for sample and reference mirror mounting.
- Implemented in situ gold or aluminum evaporation for scattering correction.
- Applied Mie theory to estimate and correct for diffraction effects.
- Interchanged sample and reference positions using a 90° rotation with mechanical stops.
Main Results:
- The technique successfully measures reflectance from 40 cm(-1) to 40000 cm(-1) between 10 K and 300 K.
- Scattering and diffraction effects were corrected, allowing for accurate measurements.
- Calculations indicate that the ratio of backscattered intensities approximates specular reflectance for samples ~1 mm in diameter.
Conclusions:
- The developed technique offers a reliable method for characterizing the optical properties of small, irregular samples.
- The approach is suitable for a wide range of materials and experimental conditions.
- This method enhances the ability to study material behavior across different spectral regions and temperatures.

