GL Spectis 1.0 Spectrometer

GL Spectis 1.0

Precise light measuring technology in a handy size.



We present the GL Spectis 1.0 for a variety of uses. This high-quality and easy to operate device gives you all you need for reliable light measurement. Check out its unique capabilities. GL Spectis 1.0 is a practical and reliable measuring device. It is ready for use immediately after connecting to your PC. No extra power supply is required. Thanks to its high sensitivity and accuracy, it is the perfect solution for light measurement. Different light sources like LED, fluorescent lamps or LCD displays require different optical probes. GL Spectis 1.0 can be combined with additional equipment to measure any type of light sources, displays as well as LED lights. Find out more about the best mini-spectrometer available on the market now! GL Spectis 1.0 optical systems and software can be easily adapted to meet any customer needs. To meet the challenges of the modern lighting industry and demanding LED market, GL Optic developed a practical hand-held spectrometer which can be used for everyday incoming quality control of light sources, field work of quality engineers and other professionals who deal with the quality of light. The GL Spectis 1.0 is a measuring device suitable for the final assessment of lamps as well as for testing of complete lighting installations. It is the perfect instrument for the measurement of LEDs.

 

UNIQUE FEATURES

  • High sensitivity and precise calibration
  • Low noise and stable measurements
  • Ready to work when connected to PC (after about 10 min)
  • Small size and low energy consumption
  • Powered via USB connection

 

USAGE

  • Different light source measurements: halogens, fluorescent lamps
  • LED measurement and testing compliant with CIE 127:2007
  • Display measurement


Practical instrument with high potential

The GL SPECTIS 1.0 optical system uses a miniature collimating lens with nano-imprint of diffraction lines and a CM OS image sensor working in the range of 340-750nm. It is a miniature low stray light system providing a 1.7nm data acquisition interval which is ideal for the measurement of LEDs, OLEDs and other light sources in the visual range. The electronic board ensures the proper speed of data transfer and very low noise. The temperature sensor installed on the board monitors the change of the ambient temperature and its influence on the measurement stability. The SP X driver software includes any necessary correction procedures to reduce stray light, bandpass error, noise level and background level to achieve the best spectra representation and highest measurement accuracy. The data acquired are calculated according to CIE norms to obtain the right color calculation for LED and other light sources.

 

TECHNICAL DATA

 

Spectral range 340-750nm / 640-1100nm
Detector CMOS image sensor
Numer of pixels 256
Physical resolution ~ 1.7nm / ~ 1.8nm
Wavelength reproducibility 0.5nm
Integration time 5ms to 100s
A/D conversion 16 bits
Signal to noise ratio 1000:1
Stray light 2*10E-3
Optical FWHM 12nm
Spectroradiometric accuracy 4%
Measurement uncertainty of color coordinates (x.y) 0.0015
Connector for optical fiber SMA905D
PC interface USB 2.0 standard
Power consumption < 100mA
Ambient temperature 5-35 °C
Dimensions 62mm x 115mm x 19/30mm
Weight 120g

 

 

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