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Title: Calculation of the optical power profile for a solar bowl with an iris

Technical Report ·
OSTI ID:5999804

This report develops analytical techniques for studying shallow spherical segment bowls that have an attached tracking iris. The report extends previous analytical models that were developed as part of the Crosbyton Solar Power Project for the case of spherical segment bowls. Three types of calculations are considered. First, effective apperture formulas are derived for a spherical segment bowl with an iris, and results are compared with the bowl without an iris. Secondly, analytical formulas are derived to determine spillage losses for shallow bowls. Finally, the powerful Ratio of Solid Angles (ROSA) computer code is extended to include solar profiles for a spherical segment bowl with iris. The report includes several plots comparing optical power concentration ratios for solar bowls with and without an iris. A complete listing of the extended code, ROSAIRIS, is given in the appendix. 29 figs.

Research Organization:
Texas Tech Univ., Lubbock, TX (USA). Dept. of Mathematics
DOE Contract Number:
AC04-83AL21557
OSTI ID:
5999804
Report Number(s):
DOE/AL/21557-T13; ON: DE89015784
Resource Relation:
Other Information: Portions of this document are illegible in microfiche products
Country of Publication:
United States
Language:
English