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Abet Technologies present the next generation of Solar Simulators, the Sun 2000 product line. A brand new optical design dramatically increases percentage of lamp output reaching the work plane. Illumination levels, per watt of lamp power, are typically 2x scale or higher as compared to other products currently available today. This leads to significant savings in electricity use and long life lamps replacement costs. These advanced instruments provide uniform illumination over 4x4, 6x6, and 8x8 inch fields. State of the art power supplies are built into the same housing as the optical unit minimizing EMI and power cable clutter. Numerous user-friendly features are designed into the Sun 2000 products. No-tools required, optics-safe lamp replacement procedure and eye-safe alignment optimization. The Sun 2000 family of Solar Simulators comes in a selection of spectral outputs to serve a broad range of research and industry needs. |
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Abet Technologies offer a wide range of technologies based around xenon arc lamp and solar simulator systems. |
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If you could instantly control the spectrum, intensity and timing of your light source, what could you achieve? Replacing light created by a frustrating assemblage of mechanical devices, OneLight Spectra improves illumination systems using a patented software-driven light engine – or Digital Light Source – to achieve an entirely new category of illumination. Employing simple-yet-powerful software, precise spectral profiles are created. Illumination, intensity and exposure duration are under your complete control. And the result is nothing short of evolutionary. - Instantaneous dynamic control over color, exposure and intensity
- Increased dynamic range of measurement
- Increased measurement sensitivity
- Sequential loading of multiple spectra
- Elimination of filters and shutters
- Elimination of repeated calibrations
- Expedited time to market for new tests and instruments
- Optimized imaging systems with reduced cost of component
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Features 150 W Xe Arc Lamp Fast F/1.0 condenser Unlimited expansion possibilities OEM ready Introduction The patent pending LS-150 is a compact, integrated, functional and stable 150 watt arc lamp based light source. The entire source, power supply, lamp, and optical compartment are housed in an extremely compact enclosure, 9 x 6 x 11 inches. The unit’s base allows mounting on inch or metric spaced optical tables with the optics centered over the hole pattern to allow for easy integration with the rest of your setup.
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The DH-2000-CAL Deuterium Tungsten Halogen Calibration Standard is a UV-NIR light source used to calibrate the absolute spectral response of a radiometric system. With the DH-2000-CAL and SpectraSuite Software, you can determine known absolute intensity values at wavelengths from 220-1050 nm. The DH-2000-CAL is specifically calibrated for use with optical fibres or a cosine corrector; the calibration data includes absolute intensities for wavelengths between 220-1050 nm at the fiber entrance port for both a bare fiber and a CC-3-UV Cosine Corrector.  |
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The DH-2000-CAL Deuterium Tungsten Halogen Calibration Standard is a UV-NIR light source used to calibrate the absolute spectral response of a radiometric system. With the DH-2000-CAL and SpectraSuite Software, you can determine known absolute intensity values at wavelengths from 220-1050 nm.
The DH-2000-CAL is specifically calibrated for use with optical fibres or a cosine corrector; the calibration data includes absolute intensities for wavelengths between 220-1050 nm at the fiber entrance port for both a bare fiber and a CC-3-UV Cosine Corrector.
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The compact, low-cost HG-1 Mercury Argon Calibration Source is a spectral wavelength calibration source for UV-VIS-Shortwave NIR spectrophotometric systems. The HG-1 produces first order mercury and argon spectral lines from 253-922 nm and second order argon lines to 1700 nm for use in performing fast, reliable spectrometer wavelength calibrations. Easily identifiable mercury and argon spectral emission lines are printed on the HG-1 housing. 
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The compact, low-cost HG-1 Mercury Argon Calibration Source is a spectral wavelength calibration source for UV-VIS-Shortwave NIR spectrophotometric systems. The HG-1 produces first order mercury and argon spectral lines from 253-922 nm and second order argon lines to 1700 nm for use in performing fast, reliable spectrometer wavelength calibrations. Easily identifiable mercury and argon spectral emission lines are printed on the HG-1 housing. |
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