By T.J.HOGAN I.R.THOMAS
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Additional resources for AISC - Design of Structural Connections 4th 1994
A variety of measurements were made during various atmospheric conditions, and it was established that the background radiation from the sky was virtually constant within about a 6θ° field of view around the sun. By rotating the Blackhouse about 30° to just barely obscure the solar disk, the noise was found to be within 2% or 3% of the noise magnitude measured when the solar disk occupied the center of the Blackhouse aperture. 2 (an approximation for the latitude of Los Angeles during the summer months).
43 RICHARD P. BOBCO The noise measurement techniques evolved during earlyshakedown tests of the facility. The requirement for "removing" the primary radiant source led to the technique of rotating the Blackhouse to obscure the solar disk. A variety of measurements were made during various atmospheric conditions, and it was established that the background radiation from the sky was virtually constant within about a 6θ° field of view around the sun. By rotating the Blackhouse about 30° to just barely obscure the solar disk, the noise was found to be within 2% or 3% of the noise magnitude measured when the solar disk occupied the center of the Blackhouse aperture.
Journal of Heat Transfer, Vol. 87, No. 3, Aug. 1965, pp. 388-396. , June 2U-26, 1968. , A General Computer Program for the Determination of Radiant Interchange Configuration and Form Factors —» CONFAC II, SID Rept. 65-10^3-2, Oct. 1965, North American Aviation, Inc<, Downey, Calif. "Ishimoto, T. , "Method of Evaluating Script F for Radiant Exchange within an Enclosure," AIAA Journal, Vol. 1, No. 6, June I963, pp. 11+28-1^29. P. , "Radiation Heat Transfer in Semigray Enclosures with Specularly and Diffusely Reflecting Surfaces," Transactions ASME, Ser.
AISC - Design of Structural Connections 4th 1994 by T.J.HOGAN I.R.THOMAS