Specular Reflection Accessories
Harrick Scientific's Specular Reflection Accessories are valuable for studies of films on metallic substrates and measurements of epitaxial film thickness by UV-Vis or FT-IR spectroscopy. A selection...
Our Glan-Taylor Polarizer has a wavelength range from 350 nm to 2300 nm. This efficient Vis-NIR polarizer is made from two calcite prisms assembled with an air spaced interface. The Glan-Taylor Polarizer is compact, making ... read more
Our Glan-Taylor Polarizer has a wavelength range from 350 nm to 2300 nm. This efficient Vis-NIR polarizer is made from two calcite prisms assembled with an air spaced interface. The Glan-Taylor Polarizer is compact, making it perfect for applications where there are space constraints. This polarizer is ideal for removing interference fringes from transmission spectra recorded at Brewster's angle and for obtaining optimum sensitivity for specullar reflectance measurements.
The polarizer is supported in a fully rotable holder on a sample slide plate and is readily mounted in-line with other accessories.
Harrick Scientific's Specular Reflection Accessories are valuable for studies of films on metallic substrates and measurements of epitaxial film thickness by UV-Vis or FT-IR spectroscopy. A selection...
Harrick's Variable Angle Specular Reflection Accessory is the industry standard for variable angle specular reflectance spectroscopy. It is ideal for specular reflection studies of films on metallic...
Our Brewster’s Angle Sample Holder allows thin films to be measured at various angles using transmission spectroscopy. Such measurements are used to extract film thickness and refractive index data...
Our Glan-Thompson Polarizer has a wavelength range from 350 nm to 2300 nm. This Vis-NIR polarizer is recommended for low-to-medium power applications (up to 2W cw) requiring a large field of view and...
Many UV-Vis spectrometers utilize gratings, resulting in a highly polarized beam passing through the sample compartment. The degree of polarization is strongly dependent on the wavelength...