We have designed a series of large aperture, high quantum efficiency optical TRAP detectors based on a unique concept developed at NIST Boulder (National Institute of Standards and Technology. We offer two models; SST-TRAP-C and SST-TRAP-D. The first is best suited for collimated or low divergence sources (<+/-10°) while the second is optimized for both collimated and divergent sources (<0.24 NA or +/-16°).
Optical TRAP detectors are intended for use in optical calibration of FO power meters, laser power meters and optical detectors. The Current Responsivity of our TRAP is determined from "physical constants" and is therefore, accurate to better than 1% from 450 to 980 nm (see "Calibration Uncertainty" in the table below). Compare this to the typical calibrated single element detector at +/-3%.
These detectors are designed into an EMI immune housing with a front bezel that includes a 1.035-40 threaded opening (THORLABS(TM) SMI) and is set to take a variety of Fiber Optic connectors, optics or alignment aids. The TRAP can be easily mounted to an optical bench with the 1/4-20 inch threaded mounting hole.
Use our SST TRAP Detector with our SST Power/Current Meter to create a complete, stand-alone, precision optical power meter.
By combining several high Quantum Efficiency photodiodes and a large, concave, broadband mirror in a multi-bounce optical configuration we can TRAP 99% of the light in the spectral range of 400 to 950 nm. The current responsivity at a particular wavelength for such a device is determined from physical constants in the equation:
RI = qνλ / hc
Where: q is the "charge of an electron"
It can be simplified for everyday use to:
RI (A/W) = νλ /1239.5
Where:
1239.5 is determined from physicalconstants (electron charge, planks constant, speed of light)
Here’s an example of how you’d calculate the RI for our TRAP at 632.8 nm:
RI @ 632.8nm = 0.99 x 632.8 / 1239.5
RI = 0.505 A/W
| . | SST-TRAP-D | SST-TRAP-C | Units | Conditions |
| Specification (@25%C) | Divergent | Collimated | . | . |
| Useable Aperture (diameter) | 7 | 7 | mm | |
| Detector Area | 1.0 | 1.0 | cm2 | |
| RI, Current Responsivity | 0.505 | 0.505 | A/W | Calculated from physical constants @ 632.8 nm |
| Calibrated Spectral Range | 400-950 | 400-950 | nm | For minimum uncertainty |
| Quantum Efficiency | > 99 | > 99 | % | From 400-950nm |
| Calibration Uncertainty | ||||
| < 1.5 | < 1.5 | % | ||
| < 5.0 | < 5.0 | % | ||
| < 1.0 | < 1.0 | % | ||
| Minimum Measureable Power | 0.1 | 0.1 | nW | |
| Maximum Power Density | 1.0 | 1.0 | mW/cm2 | |
| Field of View | +/- 14 | +/- 10 | degrees | 2mm diameter beam or smaller |
| Maximum Source Divergence (NA) | 0.24 | 0.12 | ||
| Spatial Non-Uniformity | < 0.02 | < 0.02 | % | Scanned with 1mm beam @632.8 nm |
| Price in USD | CALL or e-mail | CALL or e-mail | . | . |

The graph above compares the Current Responsivity (Ri) vs. Wavelength for our high Quantum Efficiency SST-TRAP, a 100% QE device and a single element photodiode.
Note the extremely close correlation between our TRAP and the theoretical curve. The spectral response of a single detector can vary greatly and can only be calibrated to about +/- 3% accuracy. The calibration uncertainty of our TRAP can be as low as 0.5% (see Calibration Uncertainty in the specification table)


