Lightwind S1 Series Black
Features:
Measurements in the 190-850nm
High performance concave grating optics for UV-VIS applications
Excellent spectral imaging with no mirrors for lowest possible stray light
Enhanced UV Sensitivity & Flat-field imaging for uniform resolution
No optical adjustments for extreme thermal stability and ruggedness
Research Grade Optical Performance – The Lightwind Concave UV-VIS spectrometer utilizes a 40mm diameter concave grating with aberration correction to provide the best optical performance of any compact spectrometer on the market.
Improved spectral shapes by reducing coma and astigmatism found in plane grating spectrograph designs.
Stray light reduction- The spectrograph architecture does not utilize mirrors, and therefore provides the lowest possible stray light, which is especially helpful for UV applications.
Enhanced sensitivity- due to the spectrometers ability to reduce light scatter, especially high power UV light, it can provide two to three times enhanced UV sensitivity as compared to plane grating/Czerny Turner optical configurations.
Uniform resolution – The concave grating produces a flat field on the CCD detector creating uniform resolution over the entire spectral range.
Thermal Stability- Optical bench architecture without mounting turrets and optical posts (typically in most USB spectrometers) decreases thermal expansion and contraction and increases overall system performance with temperature change
