SpectroRadiometer PDF Download

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 in units of watts per meter squared over the wavelength range in nanometers provided by the selected spectrometer model.  Currently, StellarNet offers Radiometer systems in the 200-1700nm range.  The the bottom of the page details the various ranges for each StellarNet Spectroradiometer.  The BLUE and GREEN-Wave models, BLACK-Comet concave grating model, and RED-Wave-NIR InGaAs 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.

- UV-VIS-NIR Ranges 200-1700nm
- Low cost - Ruggedized - high performance
- Shock-proof - Permanently aligned
- SpectraWiz Software included Free
- Battery packs for field measurements
- USB-2 interface to all notebook PCs

For application specific StellarNet Spectroradiometer configurations and example spectra visit the links below.

StellarNet Spectroradiometers for LED Measurement

StellarNet Spectroradiometers for Laser Measurement

StellarNet Spectoradiometers for Solar Measurement

SpectraWiz Software included FREE 
- Absolute intensity measurements watts/m²  
- µm watts/cm²
- PSD
- Lumens/m² -- LUX
- Moles per second -- PAR
- Footcandles /m2
- Radiant Flux (watts) / Luminous Flux (lumens)
- xy Chromaticity, dominant wavelength, purity
- Correlated color temperature (CCT)
- Set Power Spectral Density (PSD) range


Standard and Extended Ranges
StellarNet also has extended range spectroradiometers available to measure spectral irradiance over a wide range of wavelengths.  The EPP2000-UVN-SR spectroradiometer with CCD detector array covers a range of 200-1100nm.  The BLACK-Comet-SR super range, dual blazed, concave grating spectroradiometer offers a range of 220-1100nm while retaining all of the characteristics of a concave grating spectrometer!!! In addition, StellarNet offers a Dual Channel Spectrometer system for spectroradiometry, the Dual DSR (Detector Super Range) combines a CCD and InGaAs detector to cover a wavelength range of 200-1700nm for selected models.
 

NIST Calibrations

• Fast delivery: most systems can be calibrated and shipped within 1 week after receipt of order
   

• Absolute calibration: accuracy within 10% at detector integration setting used for calibration
   

• Certificate available: documentation with NIST traceable serial numbers.

See more StellarNet Measurement Diagrams!!

Experimental Setup for Laser, Laser Diode, and LED characterization

 

StellarNet Cosine Receptors allow collection of light with an 180 field of view using demountable diffusers with ~10% loss.  The CR1-UVN is a ½” diameter near cosine receptor using a sanded fused silica diffuser for 200-1700nm and has reduced 90° FOV and only low 7% loss.     

Cosine Receptor PDF

StellarNet Integration Spheres allow collection of light with an 180 field of view.  The IC2 is a 2" internal diameter sphere with 2 SMA connectors for illumination and collection of LED light. The input port is 5/8".  The IS4 and IS6 are 4" and 6" Sphere-Optic integration spheres with 2.5" input port with internal optowhite coating.  Mounting tripods and other accessories are available for LED measurement.

Integration Sphere PDF



NIST Calibration
The factory performs a calibration for the appropriate wavelength range from 300-850nm or 350-1100nm using an NIST traceable calibration source lamp.  This irradiance calibration service (IRRAD-CAL) is optional.  If the user has an appropriate irradiance calibration source lamp, a field re-calibration can be easily performed using the included SpectraWiz software.
 

SpectraWiz Software displaying 1931 xy chromaticity diagram measuring the color and Correlated Color Temperature (CCT) of an LED.



SpectraWiz Software allows the users to select the irradiance units. Additionally, scroll down menus allow the user to select their collection accessory in order to calculate radiant and luminous flux.

Dual DSR Spectroradiometer- Halogen-lamp spectra -  (300-1700nm)

Low Light Configurations-
Many popular applications involve measuring the irradiance of light sources with low output intensities. From ambient streetlight to UV-LEDs many people need to detect low levels of radiation. StellarNet spectrometers can be specially configured to measure these low light levels.  The spectrometer aperture or slit can be adjusted to allow more light into the unit, thus making it more sensitive to radiation.  For low light applications a 200um slit is the standard slit size.  Additionally, low light level calibrations can be employed to further optimize the spectrometers ability to see low light levels.  And lastly, a TEC cooler can be installed on the detector array to increase the signal to noise of the unit by 66%.  This in affect allows the spectrometer to integrate over longer periods of time, collecting more and more photons, while keeping a low noise value. If you have a low light application be sure to talk to a StellarNet sales engineer to discuss the configuration of your spectrometer.       

Bright Light Configurations-
In contrast, many industries require the measurement of really bright light emission. StellarNet spectrometers have a dynamic range of 6 decades allowing integration times from 1ms to 65s. StellarNet spectrometers can be specially configured for high power applications. The limitation of a high power radiometer will be limited by the power of the calibration source. StellarNet can configure Spectroradiometers to optimize calibration thus allowing the use of the units large dynamic range and detector linearity to allow high power light measuremnt. Additionally, smaller slits, fibers, and integration spheres can be employed to decrease the signal to the spectrometer.  StellarNet offers a high light level calibration to further optimize the system performance.