A High-Emissivity Blackbody with Large Aperture for Radiometric Calibration at Low-Temperature
- 125 Downloads
A newly designed high-emissivity cylindrical blackbody source with a large diameter aperture (54 mm), an internal triangular-grooved surface, and concentric grooves on the bottom surface was immersed in a temperature-controlled, stirred-liquid bath. The stirred-liquid bath can be stabilized to better than 0.05°C at temperatures between 30 °C and 70 °C, with traceability to the ITS-90 through a platinum resistance thermometer (PRT) calibrated at the fixed points of indium, gallium, and the water triple point. The temperature uniformity of the blackbody from the bottom to the front of the cavity is better than 0.05 % of the operating temperature (in °C). The heat loss of the cavity is less than 0.03 % of the operating temperature as determined with a radiation thermometer by removing an insulating lid without the gas purge operating. Optical ray tracing with a Monte Carlo method (STEEP 3) indicated that the effective emissivity of this blackbody cavity is very close to unity. The size-of-source effect (SSE) of the radiation thermometer and the effective emissivity of the blackbody were considered in evaluating the uncertainty of the blackbody. The blackbody uncertainty budget and performance are described in this paper.
KeywordsCylindrical blackbody Emissivity Size-of-source effect
Unable to display preview. Download preview PDF.
- 1.Quinn T.J.: High Temp.-High Press. 12, 359 (1980)Google Scholar
- 3.“STEEP 3 Version 1.3” User’s Guide, Virial. IncGoogle Scholar
- 4.http://jp.hamamatsu.com/index; P5968–060 datasheet
- 5.Y. Kaneko, Y. Shimizu, J. Ishii, in Proceedings of SICE Annual Conference, vol. 2 (The Society of Instrument and Control Engineers, Tokyo, Japan, 2004), pp. 1764–1767 (IEEE Catalog Number: 04TH8773, ISBN 4-907764-22-7). http://ieeexplore.ieee.org/iel5/9985/32062/01491716.pdf?isnumber=32062&prod=CNF&arnumber=1491716&arSt=+1764&ared=+1767+vol.+2&arAuthor=Kaneko%2C+Y.%3B+Shimizu%2C+Y.%3B+Ishii%2C+J.