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if the measurement range of KRISS is wider than that of<br />

TKK, the data measured beyond the measurement range of<br />

TKK affect the ccf within a part in 10 6 . The difference of<br />

the ccf for the illuminant A is 0.28 %, which exceeds the<br />

standard uncertainty denoted in the parenthesis in Table 1.<br />

The difference of the absolute responsivity at 555 nm<br />

is -0.3 %. Considering the degree of equivalence of the<br />

spectral responsivity between both institutes, -0.12 % at<br />

550 nm [5], we can see that an additional difference,<br />

-0.18 %, though much smaller than its standard uncertainty<br />

of 0.40 %, has appeared in the responsivity comparison.<br />

The aperture area measurements are compared using<br />

four apertures with diameters of 5 mm, 7 mm and 8 mm.<br />

For all apertures, the relative area difference of KRISS and<br />

TKK is between -0.005 % and -0.048 %. The area<br />

measured by TKK and its difference with KRISS shown in<br />

Table 1 is estimated from the area comparison result for<br />

the aperture which has the same diameter as the aperture<br />

attached in the artifact photometer.<br />

The final difference of the illuminance responsivity of<br />

the artifact is -0.6 %, which mainly comes from<br />

contributions of difference of the responsivity at 555 nm<br />

and of the ccf for the illuminant A. The aperture area<br />

difference is somewhat larger than the standard uncertainty,<br />

but its contribution to the illuminance responsivity<br />

difference is almost negligible.<br />

Table 1. Comparison of quantities obtained during realization of<br />

the illuminance responsivity for the artifact. The numbers in the<br />

parentheses correspond to the standard uncertainty.<br />

Quantities KRISS TKK<br />

Responsivity at<br />

555 nm (A/W)<br />

Aperture<br />

(cm 2 )<br />

area<br />

ccf for<br />

illuminant A<br />

Illuminance<br />

responsivity<br />

(nA/lx)<br />

KRISS-TKK<br />

0.1974(6) 0.1980(4) -0.3(4) %<br />

0.38492(6) 0.38507(10) -0.04(3) %<br />

0.9958(14) 0.9930(12) 0.28(19) %<br />

11.17(4) 11.24(3) -0.6(4) %<br />

III. Comparison of illuminance responsivity<br />

At TKK, the illuminance scale is not realized by using<br />

the above procedure, but by using trap-detector based<br />

photometers, for which the V(λ) filter is separately<br />

measured in terms of spectral transmittance.[3] The<br />

spectral responsivity of the trap detector is also calibrated<br />

traceable to the cryogenic radiometer. The radiometric<br />

aperture area is measured by GBS.[2]<br />

The TKK reference photometer was compared with the<br />

artifact photometer at TKK. The artifact drift during the<br />

comparison period and transportation was checked after<br />

return to KRISS and revealed to be insignificant. The<br />

difference in the illuminance scales was -0.1 %, with an<br />

expanded uncertainty of 0.9 %, which is much smaller<br />

than the difference of -0.6 % shown in Table 1. However,<br />

the differences are within combined standard uncertainties<br />

of the comparisons. In another illuminance responsivity<br />

comparison the difference between KRISS and TKK was<br />

-0.2 % with an expanded uncertainty of 0.6 % [6].<br />

Considering these facts, the deviation of -0.6 % of Table 1<br />

is acceptable. However, both institutes seem to be<br />

somewhat too optimistic with the uncertainty estimates.<br />

IV. Conclusions<br />

The illuminance scales realized and maintained at<br />

KRISS and TKK have been compared to show a good<br />

agreement between 0.1 and 0.2 %. TKK was asked to yield<br />

the illuminance responsivity of the artifact photometer<br />

supplied by KRISS according to the KRISS procedure.<br />

The illuminance responsivity given by TKK using the<br />

KRISS procedure is 0.6 % higher than that given by<br />

KRISS. Considering the uncertainties of the measurements,<br />

the difference is acceptable. However, since both institutes<br />

seem to be somewhat too optimistic with the uncertainties<br />

of the ccf and the aperture area, the uncertainties may need<br />

to be addressed to cover these deviations.<br />

References<br />

[1] Khler R., Stock M. and Garreau C., Final Report on<br />

the International Comparison of Luminous Responsivity<br />

CCPR-K3.b, Metrologia 41, Tech. Suppl., 02001, 2004.<br />

[2] Ikonen E., Toivanen P. and Lassila A., A new optical<br />

method for high-accuracy determination of aperture area,<br />

Metrologia 35, 369, 1998.<br />

[3] Kh P., Haapalinna A., Toivanen P., Manoochehri F.<br />

and Ikonen E., Filter radiometry based on direct<br />

utilization of trap detectors, Metrologia 35, 255, 1998.<br />

[4] Manoochehri F., Kärhä P., Palva L., Toivanen P.,<br />

Haapalinna A., and Ikonen E., Characterization of<br />

Optical Detectors Using High-Accuracy Instruments,<br />

Anal. Chim. Acta 380, 327 (1999).<br />

[5] Goebel R. and Stock M., Report on the comparison<br />

CCPR-K2.b of spectral responsivity measurements in<br />

the range 300 nm to 1000 nm, Metrologi, 41, Tech.<br />

Suppl.,02004, 2004.<br />

[6] Ikonen E. and Hovila J., Final Report of<br />

CCPR-K3.b.2-2004: Bilateral Comparison of<br />

Illuminance Responsivity Scales between the KRISS<br />

(Korea) and the HUT (Finland), Metrologia 41, Tech.<br />

Suppl. 02003, 2004.<br />

326

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