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Characterization of Thermopile for Laser Power Measurements<br />

A. K. Türkoğlu<br />

Ulusal Metroloji Enstitüsü, Kocaeli, Turkey<br />

Abstract. Due to their high wavelength and power range,<br />

thermal detectors were employed in our measurement<br />

set-up for optical power measurements. A link between<br />

optical power calibrations at medium power levels and our<br />

primary standard cryogenic radiometer was established by<br />

means of transfer standards. Analysis of the set-up and<br />

characterization of our working standard thermal detectors<br />

to yield uncertainty budget is presented in this study.<br />

Detector Based Measurements<br />

As the needs and applications of optical measurements<br />

increase, we frequently face with new radiation detectors<br />

and lasers with different structure, speed, range or beam<br />

properties. However in the calibration and measurements,<br />

commercially, there is no single suitable working standard<br />

detector available to cover all the power and optical<br />

wavelength range of interest.<br />

In our laboratory, treaceability from our Cryogenic<br />

Radiometer (Oxford Instr., Radiox) is provided by using a<br />

set of home-built 3-element reflection type trap detectors<br />

as the transfer standards. Due to the type of silicon<br />

detectors used, those trap detectors can be used safely in<br />

300 to 1100 nm wavelength range but only up to 3 mW<br />

incident power due to their linearity limits. The<br />

measurements at wider wavelength ranges have become<br />

possible by employing our Electrically Calibrated<br />

Pyroelectric Radiometer. But for higher power ranges, it<br />

was found out that it is not feasible to use filtered<br />

photodetectors due to the heating effects, nonhomogeneity<br />

of the filter surface and strong depen- dence of the<br />

alignment and on incident angle. Therefore, we have<br />

chosen and employed thermopiles in our laser power<br />

measurement and detector calibration set-up.<br />

Laser Sources<br />

Our monochromatic line source facility contains an 11<br />

mW HeNe of 632.8 nm and a 20 mW Tunable Argon<br />

lasing at 488 and 514 nm. For medium power ranges, we<br />

added an intensity stabilized 2W Nd-YAG laser to our<br />

set-up, which has a main beam at 1064 nm wavelength and<br />

an additional green line at 532 nm.<br />

Detectors<br />

For internal checks and dissemination, we have used<br />

filtered UV and Ge detectors which are capable up to<br />

optical powers of 30 mW. We have added three<br />

thermopiles with 3, 30 and 250 W maximum optical power<br />

thresholds to our measurement facility. Circular active<br />

areas of the thermopiles were defined with the diameters of<br />

12, 18 and 50 mm respectively. Selected detectors had<br />

response times of 0.8 to 2.5 s. These detectors were chosen<br />

especially for their good repeatibility, spatial uniformity<br />

and rather flat responsivity over a wide range which was<br />

stated as 0.2 to 20 µm.<br />

Figure 1. Reflectance Curve of Thermopile Coating<br />

Characterization<br />

For the flatness of the spectral responsivity, the<br />

diffuse reflectance of the thermopile was measured by<br />

mono- chromator and found to be as 95,2 ± 1,2 % between<br />

200 and 800 nm. Reflectances at single laser lines were<br />

also measured seperately as shown in Fig.1.<br />

Nonlinearity behaviour was studied by means of<br />

detector sensitivity measurements taken at eight different<br />

levels and found to be increasing up to 0.4 % level as<br />

optical power goes to 1.6 W. Homogeneity of sensitivity<br />

was analyzed 7 mm around the center and detected as<br />

below 0.25 % except for the largest area detector. The<br />

stray light and divergence effects was also measured to be<br />

very low, around 0.05 % for nominal 60 cm measurement<br />

distance on the set-up. Over 100 mW level, random power<br />

fluctuations by the source were seen to be more effective<br />

than the any other factor, and therefore were tried to be<br />

minimized by employing a monitor detector.<br />

Results<br />

A thermopile based laser power measurement set-up<br />

working at medium power levels from visible to near<br />

infrared range has been established. Responsivity, linearity<br />

and uniformity focused analysis resulted that<br />

measurements at an uncertainty level (k=2) of 1.4 % for<br />

the visible range (up to 20 mW) and of 1.9 % in the<br />

infrared (for 1.6 W at 1064 nm), have become possible by<br />

this power and wavelength range extension study.<br />

References<br />

Li, X., T. R. Scott, C. L. Cromer, D. Keenan, F. Brandt, K.Möstl,<br />

Power Measurement Standards for High-Power Lasers:<br />

Comparison between the NIST and the PTB, Metrologia, 37,<br />

pp.445-447, 2000.<br />

Li, X., T. Scott, S. Yang, C. Cromer, M. Dowell, Nonlinearity<br />

Measurements of High-Power Laser detectors at NIST,<br />

Journal of Research of the NIST, 109, No.4, pp429-434, 2004.<br />

Möstl, K., Laser Power and Energy Radiometry, Institute of<br />

Physics, Conference Series, No.92, pp.11-18, London, 1988.<br />

Turkoglu, K., F. Samadov, M. Durak, U. Kucuk, Construction of<br />

a Reference Photometer Head for the Realization of Candela,<br />

Proceedings of CIE Congress, Volume II, pp. 379-386,<br />

Proceedings NEWRAD, 17-19 October 2005, Davos, Switzerland 329

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