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Title: Spectral emissivity of tungsten: analytic expressions for the 340-nm to 2. 6-. mu. m spectral region

Journal Article · · Appl. Opt.; (United States)
DOI:https://doi.org/10.1364/AO.23.000975· OSTI ID:5461821

To correct emission spectra a standard radiance source is often used to determine the spectral responsivity of the detection system. In the near-UV, visible, and near-IR spectral regions the most common radiance standard is a tungsten strip lamp calibrated by a standards laboratory. For day-to-day experiments where slightly less accuracy is acceptable, a less expensive uncalibrated lamp is useful. In this case, the radiant temperature T/sub r/ of the lamp is measured with an optical pyrometer, generally at a single wavelength such as 650 nm, and the source spectral radiance L(lambda) is calculated from L(lambda) = tau(lambda)epsilon(lambda,T)L/sub B/(lambda,T). The transmittance of the source is tau(lambda), the spectral emissivity is epsilon(lambda,T), and L/sub B/(lambda,T) is the spectral distribution of blackbody radiation, Planck's radiation law. To obtain the true temperature T, Wien's approximation is employed. To conveniently calibrate a system, especially one which utilizes a microcomputer, it is advantageous to have analytic expressions for the spectral emissivity of tungsten. Although Larrabee has published such expressions, they are limited to the 450-800-nm spectral region. To obtain analytic expressions from 340 nm to 2.6 ..mu..m they have used the measurements of DeVos. Although DeVos's results differ by 2% from those of Larrabee, this difference is assumed to be acceptable.

Research Organization:
Argonne National Lab., IL
DOE Contract Number:
W-31-109-ENG-38
OSTI ID:
5461821
Journal Information:
Appl. Opt.; (United States), Vol. 23:7
Country of Publication:
United States
Language:
English