Description
The StellarNet model spectrometers are great tools for low cost, routine analysis of all types of light. From measuring the irradiance of standard light bulbs to measuring the exact color coordinates of the yellow in a traffic light, StellarNet spectrometers are used worldwide to routinely analyze light. These instruments are calibrated to measure the spectral irradiance, radiance, or Watt flux over the wavelength range in nanometers provided by the selected spectrometer model.Currently, StellarNet offers Radiometer systems in the 200-1700nm range!
SpectraWiz Software can calculate many important values such as lumens, xy chomaticity, dominant wavelength, Correlated Color Temperature (CCT), and much more.
There are various ranges for each StellarNet Spectroradiometer. The BLUE and GREEN-Wave models, BLACK-Comet concave grating model, and RED-Wave-NIRInGaAs model can be configured to have the correct slit size and detector array to suite your application. Calibrated spectroradiometers can be used to measure absolute intensity, xy Chromaticity (CIE 1931), purity, correlated color temperature, and dominant wavelength.
SpectroRadiometer Test Reporting Software-
The SpectroRadiometer Test Report Software now enables customers to prepare and instantly display all of the relevant test data on one sheet making quality control and R&D efforts much more efficient. Instantly acquire a complete spectrum of your test light source and view its color distribution with an under the curve wavelength color representation. This spectral curve allows for easy identification of color distribution of your light source.
- Total Power (Watts and Lumens)
- Efficiency & Efficacy
- CIELAB with the xy/u’v’ chromaticity
- CCT (Correlated Color Temperature)
- PAR
- Dominant wavelength
- Percent color purity.
- CRI (Color Rendering Index)
- CQS (Color Quality Scale)
The DWARF STAR and BLUE WAVE spectroradiometer configuration is a sophisticated setup designed for comprehensive spectral analysis across a wide range of wavelengths. This configuration combines two advanced spectroradiometers, each optimized for different segments of the electromagnetic spectrum, providing a complete and precise spectral profile from UV to IR.
The BLUE WAVE is a versatile UV-VIS-NIR spectroradiometer that excels in its portability, durability, and high-resolution performance. Featuring a 2048-element CCD detector with 16-bit resolution, it ensures highly accurate real-time measurements. This lightweight device is powered via USB2, making it convenient for fieldwork and laboratory settings alike. Its broad wavelength range allows for detailed analysis of light in the ultraviolet, visible, and near-infrared spectra, making it an invaluable tool for a variety of scientific and industrial applications.
The DWARF STAR NIR-IR Spectroradiometer is a specialized NIR-IR spectroradiometer that complements the BLUE WAVE by covering the near-infrared to infrared spectrum. It is equipped with a 512-element InGaAs detector, providing high sensitivity and accuracy. The DWARF STAR is continuously cooled with its temperature precisely maintained at -10°C, ensuring stable and reliable performance. This device is also portable and lightweight, powered by both a power supply and USB2, which enhances its flexibility for various measurement environments.
Integrated Measurement with SpectraWiz Software
The SpectraWiz software plays a crucial role in the DWARF STAR and BLUE WAVE configuration by seamlessly integrating the two instruments. Connected via a specialized Y-shaped optical fiber, the software combines the spectra from both devices into a single, comprehensive spectral profile. This integration enables users to obtain a complete spectrum spanning from ultraviolet to infrared wavelengths, thus providing an extensive analysis tool for a wide range of scientific and industrial applications.
In summary, the DWARF STAR and BLUE WAVE configuration, enhanced by SpectraWiz software, offers a powerful and versatile solution for precise spectral measurement across the UV to IR spectrum. Ideal for researchers and professionals needing detailed spectral data, this setup combines advanced technology with ease of use for exceptional analytical capabilities.
