Updated:2025-01-07
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Gentec-EO IS12L-9S-RSi-INT-D0 Integrating sphere detector for laser power measurement up to 9 W.
Measure from low powers to the multi-kilowatt level with a single device
The broad dynamic range and very low noise equivalent power (NEP) of the IS integrating spheres provide users the ability to measure several lasers with different average powers with only one device.
Outstanding signal-to-noise ratios (SNR)
No need to change detector or manage attenuation when the measured power spans a wide range
Lower initial and maintenance costs compared to buying multiple detectors to cover the same range
Monitor high-power lasers at high speed
Thanks to their photodiode-based sensor, power meters of the IS series measure in under 200 ms, tens of times faster than with thermal detectors.
Faster measurements: no need to wait for the detector to stabilize
Discern quick changes in laser power
Follow the ramp-up of high-power sources
Increased productivity
Diffused back-reflections confined in an angular cone
While thermal detectors and water calorimeters diffusely reflect 10% to 15% of the incoming light in a Lambertian manner, integrating spheres of the IS series reflect only 6% to 12% more directionally through their optical aperture. This helps improve safety in the measurement environment by making it easier to deal with back reflections.
Fast response in the VIS-NIR range with a silicon absorber and the IS series
Photodiode-based detector offering a fast response for VIS-NIR wavelength. Our silicon absorber makes it possible to measure very low powers down to the microwatt level. Its damage thresholds are higher than any other “white” coatings on the market.
Outstanding dynamic range
Fast response
Reduced angular back-reflections
High damage thresholds
Optional INTEGRA (USB or RS-232) output
When you choose the INTEGRA output option you get an all-in-one measurement instrument that combines both the detector and the meter in one convenient product. Plug the detector in your PC, install our free software and start measuring.
The most cost-efficient solution
Same measurement performance as our other solutions
No compromise on interface functions and features
Compact solution for OEM applications and field servicing
Save money on recalibration with an all-in-one instrument
Key Features
High average power
12 mm aperture for up to 9 W of continuous power
50 mm aperture for up to 1000 W of continuous power
Resistant coating
Our proprietary coating is designed to be strong. Its damage thresholds are orders of magnitude higher than any other "white" coatings on the market.
Precise calibration
The IS detectors have a NIST-traceable calibration for their entire calibrated spectral range. Temperature compensation completes the calibration to give you the most accurate and stable measurements.
Choice of output
The IS detectors are available with two output options:
INTEGRA with USB output (-INT)
INTEGRA with RS-232 output (-IDR)
Specifications
Measurement capabilities | |
Maximum average power (continuous) | 9 W |
Noise equivalent power | 1 μW |
Spectral range | 340 - 1100 nm |
Typical rise time | 0.2 s |
Linearity with power | ±1 % |
Sphere inner diameter | 50 mm Ø |
Maximum incidence angle | ± 10° |
Maximum divergence | 10° (half-angle) |
Power calibration uncertainty |
±5.0 % (405 - 499 nm) ±3.5 % (500 - 1063 nm) ±2.5 % (1064 nm) |
Calibrated spectral range | 405 - 1070 nm |
Back reflections | 6 %, concentrated in a cone with 7.5 degrees half-angle |
1. At 1070 nm. Nominal value. Actual value depends on environmental electromagnetic interference and wavelength. | |
Damage thresholds | |
Maximum average power density | 2 kW/cm² |
Maximum energy density | 400 mJ/cm² |
1. At 1064 - 1070 nm, CW. May vary with wavelength and average power. 2. At 1064 - 1070 nm, 7 ns. May vary with wavelength and pulse width. |
|
Physical characteristics | |
Cooling | Convection |
Aperture diameter | 12 mm |
Dimensions | 66H x 78W x 66D mm |
Weight | 0.7 kg |
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