Mar 19, 2017 | Glossary of Spectroscopy Terms, Spectrograph
Plane (flat) gratings are prone to coma and astigmatism. Using multiple optics, as in the Czerny-Turner configuration, also increases the stray light. To minimize these errors, the BLACK-Comet spectrometer uses a concave grating. This means the three optics in a...
Mar 19, 2017 | Glossary of Spectroscopy Terms, Spectrograph
The Czerny-Turner configuration is a specific arrangement of optics in spectrographs. There are other configurations, but Czerny-Turner is the most common. A majority of StellarNet spectrometers use the Czerny-Turner configuration. The diagram below shows the...
Mar 19, 2017 | Glossary of Spectroscopy Terms, Properties of Light, Spectrograph
Chromatic aberration is an aberration caused by dispersion. When a beam of light is transmitted through a lens, dispersion causes the wavelengths to focus at different focal points. The aberration can be corrected by adding other materials to essentially cancel out...
Mar 19, 2017 | Glossary of Spectroscopy Terms, Properties of Light, Spectrograph
An aberration is when an optical system deviates from the expected ideal outcome. For example, lenses are expected to focus all rays of light to a single focal point. In practice, no lenses accomplish this. The cause of the deviation is called an aberration. In...
Mar 19, 2017 | Glossary of Spectroscopy Terms, Spectrograph
The wavelength range (also called spectral range) is the range of wavelengths that each spectrometer can measure. StellarNet offers spectrometer options that cover a 190-2500nm wavelength range. Wavelength range is based on the spectrometers grating’s ability...
Mar 19, 2017 | Glossary of Spectroscopy Terms, Spectrograph
Also called a grating for short, a diffraction grating is by far the most common dispersive element in spectrographs these days. As might be guessed, diffraction gratings work through diffraction. The gratings can be transmissive or reflective, but the principles are...