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Realization of the NIST total Spectral Radiant Flux Scale - PMOD/WRC

Realization of the NIST total Spectral Radiant Flux Scale - PMOD/WRC

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where y test (λ) is <strong>the</strong> detector signal <strong>of</strong> <strong>the</strong><br />

spectroradiometer for <strong>the</strong> test lamp at wavelength λ, and<br />

y ref (λ) is that for <strong>the</strong> introduced flux at wavelength λ.<br />

k cor (λ) is a correction factor for spatial nonuniformity <strong>of</strong><br />

<strong>the</strong> integrating sphere system and <strong>the</strong> ratio <strong>of</strong> diffuse<br />

reflectance <strong>of</strong> <strong>the</strong> sphere coating at 0° and 45° incidence.<br />

Similar to <strong>the</strong> case with <strong>the</strong> goniospectroradiometric<br />

method, <strong>the</strong> measurement can be done for relative <strong>total</strong><br />

spectral radiant flux, with <strong>the</strong> absolute scale determined by<br />

<strong>the</strong> luminous flux unit.<br />

Instrumentation<br />

The mechanical design <strong>of</strong> <strong>the</strong> goniospectroradiometer<br />

developed at <strong>NIST</strong> is shown in Fig. 1. The detector arm<br />

and lamp holder are rotated by servo motors, and <strong>the</strong> actual<br />

angles are measured by rotary encoders. Measurements are<br />

taken, typically at 5° or 10° intervals, and <strong>the</strong> motor stops<br />

during measurement. The arm holding <strong>the</strong> lamp holder can<br />

also be rotated to change <strong>the</strong> burning position <strong>of</strong> <strong>the</strong> lamp.<br />

The spectral irradiance <strong>of</strong> <strong>the</strong> test lamp is measured with<br />

an array spectroradiometer employing a fiber optic input.<br />

The fiber bundle is connected to <strong>the</strong> spectroradiometer<br />

through a rotation coupler, which allows free rotation <strong>of</strong><br />

<strong>the</strong> arm without twisting <strong>the</strong> fiber. The constancy <strong>of</strong> <strong>the</strong><br />

spectral transmittance <strong>of</strong> <strong>the</strong> coupler was tested with a<br />

white LED mounted on <strong>the</strong> irradiance head. The variations<br />

in measured spectra depending on <strong>the</strong> arm angle was found<br />

to be less than 2 %, and is corrected in actual<br />

measurements. From <strong>the</strong> rotation coupler to <strong>the</strong> irradiance<br />

measuring head, a fiber bundle <strong>of</strong> 8 mm diameter is used.<br />

The fiber bundle on <strong>the</strong> spectroradiometer side is 5 mm<br />

diameter.<br />

The array spectroradiometer covering <strong>the</strong> UV and visible<br />

region is calibrated by a spectral irradiance standard lamp<br />

(1000 W FEL type quartz halogen lamp) traceable to <strong>the</strong><br />

<strong>NIST</strong> spectral irradiance scale [7]. The stray light <strong>of</strong> <strong>the</strong><br />

array spectrometer has been corrected (Zong, 2005). For<br />

<strong>the</strong> consistency with <strong>the</strong> <strong>total</strong> luminous flux unit, <strong>the</strong> <strong>total</strong><br />

spectral radiant flux scale has been realized using Eqs.<br />

Servo<br />

motor<br />

Stepping<br />

motor<br />

Irradiance<br />

head<br />

1.25 m<br />

φ<br />

Light<br />

trap<br />

Encoder<br />

Laser<br />

Servo<br />

motor<br />

Fiber<br />

bundle<br />

Figure 1. Construction <strong>of</strong> <strong>the</strong> <strong>NIST</strong><br />

goniospectroradiometer.<br />

θ<br />

Spectroradiometer<br />

Rotation<br />

coupling<br />

Figure 2. <strong>NIST</strong> 2.5 m integrating sphere configured<br />

for <strong>the</strong> <strong>total</strong> spectral radiant flux measurement.<br />

(3)-(5). The uncertainty budget is to be reported at<br />

presentation and <strong>the</strong> full paper.<br />

Figure 2 shows <strong>the</strong> arrangement <strong>of</strong> <strong>the</strong> <strong>NIST</strong> 2.5 m sphere<br />

configured for <strong>total</strong> spectral radiant flux measurement.<br />

The sphere is equipped with a high-sensitivity<br />

spectroradiometer employing a back-lit CCD array. The<br />

external source is a 1000 W FEL type quartz halogen lamp<br />

calibrated for spectral irradiance. The aperture is 50 mm in<br />

diameter. The spectroradiometer is an array<br />

spectroradiometer, which is corrected for stray light (Zong,<br />

2005). Linearity <strong>of</strong> <strong>the</strong> spectroradiometer has also been<br />

determined and corrected. The integrating sphere response<br />

has been mapped spectrally by rotating a beam scanner.<br />

Angular correction factor for <strong>the</strong> coating has also been<br />

measured spectrally. An experimental realization <strong>of</strong> <strong>total</strong><br />

spectral radiant flux scale in <strong>the</strong> near UV region (360 nm –<br />

450 nm) has been successfully made at <strong>NIST</strong> using <strong>the</strong> 2.5<br />

m integrating sphere to calibrate <strong>the</strong> <strong>total</strong> radiant flux <strong>of</strong><br />

deep blue and UV LEDs (Zong, 2004). Work is underway<br />

to realize <strong>the</strong> scale in <strong>the</strong> full visible region.<br />

Conclusion<br />

The <strong>total</strong> spectral radiant flux scale has been established at<br />

<strong>NIST</strong> using a goniospectroradiometer for <strong>the</strong> 360 nm to<br />

800 nm region. The AIS method, now under development,<br />

will enable realization <strong>of</strong> <strong>the</strong> scale with much simpler<br />

instrumentation and fast measurements.<br />

References<br />

Goodman T. M., et al, The Establishment <strong>of</strong> a New National<br />

<strong>Scale</strong> <strong>of</strong> <strong>Spectral</strong> Total <strong>Flux</strong>, Proc., 22 nd Session <strong>of</strong> CIE,<br />

Melbourne 1991, Vol. 1, Part 1, 50-53 (1991).<br />

CORM 7 th Report 2001–Pressing Problems and Projected<br />

National Needs in Optical Radiation Measurements, December<br />

2001.<br />

Ohno Y., <strong>Realization</strong> <strong>of</strong> <strong>NIST</strong> 1995 Luminous <strong>Flux</strong> <strong>Scale</strong> using<br />

Integrating Sphere Method, J. IES, 25-1, 13-22 (1996).<br />

Zong, Y., et al, A Simple Stray-light Correction Matrix for Array<br />

Spectrometers, to be presented at NEWRAD 2005<br />

Zong, Y., Miller, C.C., Lykke, K., Ohno, Y., Measurement <strong>of</strong><br />

Total <strong>Radiant</strong> <strong>Flux</strong> <strong>of</strong> UV LEDs, Proceeding <strong>of</strong> <strong>the</strong> CIE Expert<br />

Symposium on LED Light Sources, June 2004, Tokyo,<br />

107-110 (2004)

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