Ophir Optronics Ltd QSR Manual Do Utilizador
Appendix B – Calibration, Traceability, and Recalibration
Ophir Thermopile Heads
Figure B-2 Absorption vs. Wavelength of Pyroelectric and Excimer Head Absorbers
Factory Calibration of Thermopile Heads
The absorption of the various Ophir thermal absorbers can vary from disc to disc.
Therefore, all Ophir absorbers are individually calibrated against NIST traceable
standards. Ophir power/energy meters with the broadband or P type absorbers
are individually calibrated by laser at several wavelengths against a NIST
calibrated standard meter. The meter can be switched to give the exact
calibration at the various wavelengths, for example, Argon, YAG, and where
applicable, CO2.
Therefore, all Ophir absorbers are individually calibrated against NIST traceable
standards. Ophir power/energy meters with the broadband or P type absorbers
are individually calibrated by laser at several wavelengths against a NIST
calibrated standard meter. The meter can be switched to give the exact
calibration at the various wavelengths, for example, Argon, YAG, and where
applicable, CO2.
The EX type detector is calibrated by measuring the ratio of absorption in the
UV to that at 515nm. In both cases, the total absorption is measured using an
integrating sphere. The detector is then calibrated with an argon laser and given a
correction factor from this ratio.
UV to that at 515nm. In both cases, the total absorption is measured using an
integrating sphere. The detector is then calibrated with an argon laser and given a
correction factor from this ratio.
Linearity and Accuracy of Thermopile Heads
Linearity
The linearity of most Ophir thermal detectors is specified to be 1% over the
specified power range of each particular instrument, and is periodically tested by
Ophir.
specified power range of each particular instrument, and is periodically tested by
Ophir.
For models whose linearity is not tested over their entire range, samples are
randomly chosen and periodically tested over their entire range. The test is
performed with a high power laser that covers the entire detector range using a
rear leak detector for comparison. The rear leak detector is a low power Ophir
detector that has previously been tested for linearity. In all cases, the linearity of
the detectors is traceable to electrical standards.
randomly chosen and periodically tested over their entire range. The test is
performed with a high power laser that covers the entire detector range using a
rear leak detector for comparison. The rear leak detector is a low power Ophir
detector that has previously been tested for linearity. In all cases, the linearity of
the detectors is traceable to electrical standards.
StarLab User Guide
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