1960
DOI: 10.6028/jres.064a.028
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Standard of spectral radiance for the region of 0.25 to 2.6 microns

Abstract: This papr r co nlain information relatin g to t hg setting L~P <;>f s lalldarc~ b lackbodi es [~r use t hro ug h t he te mperat ure range of abo ut 1,400 to 2,400 h and then use In the caIJbration of tungste n strip lamps as Iaboratory .stand a rds of spectral . rad Ia nce fO I· t he lVit;-relength regio n of 0.25 to 2.6 mi crons. A gml?h lte b lackbody IS d esc n bed a nd rep rese ntatlvr data a re gi ven on the spec tnd c ha racte l'ls tlCs of the new lamp standard as compared to b la ckbodies at se veral se… Show more

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Cited by 80 publications
(10 citation statements)
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“…After fairly successful use for more than half a century, [60][61][62][63][64] conventional tungsten ribbon lamps 19 calibrated against NIST standards for absolute values of spectral radiance were discontinued. The modern alternatives to these relatively cheap yet robust and reliable light sources are standards of spectral radiance employing integrating spheres 65,66 and high-power quartz halogen lamps or quasi-continuouswave lasers.…”
Section: Continuous Laboratory Sourcesmentioning
confidence: 99%
“…After fairly successful use for more than half a century, [60][61][62][63][64] conventional tungsten ribbon lamps 19 calibrated against NIST standards for absolute values of spectral radiance were discontinued. The modern alternatives to these relatively cheap yet robust and reliable light sources are standards of spectral radiance employing integrating spheres 65,66 and high-power quartz halogen lamps or quasi-continuouswave lasers.…”
Section: Continuous Laboratory Sourcesmentioning
confidence: 99%
“…The greatest source of error in the use of tungsten lamps appears to be the un cer· tainty in the spectral emissivity (e(A» of tungsten. T o overcome this error, Stair et al [24] at the National Bureau of Standards, Washington, D.C., individually calibrate tungsten strip lamps against a high temperature black body, and it is probable that these lamps (type U90) are the most accurate spectral radiant sources presently available. The uncertainty in output ranges from a maximum of 8 percent at short wavelengths to 3 percent at long wavelengths [24].…”
Section: B Tungsten Lamp Calibrationmentioning
confidence: 99%
“…T o overcome this error, Stair et al [24] at the National Bureau of Standards, Washington, D.C., individually calibrate tungsten strip lamps against a high temperature black body, and it is probable that these lamps (type U90) are the most accurate spectral radiant sources presently available. The uncertainty in output ranges from a maximum of 8 percent at short wavelengths to 3 percent at long wavelengths [24]. A description of the use of a standard tungsten lamp is given by Christiansen and Ames [25].…”
Section: B Tungsten Lamp Calibrationmentioning
confidence: 99%
“…(1) replacement of the system source by a 'standard source', such as a calibrated tungsten bulb (Stair, Johnston & Halbach, 1960); (2) replacement of the system detector by an absolute detector, such as a thermopile (Melhuish, 1972;Rutgers, 1972); (3) use of a quantum counter of known quantum efficiency (Melhuish, 1972).…”
Section: Photon-cozmting Chainmentioning
confidence: 99%