WIND LOADING ON SOLAR COLLECTORS

by UNIVERSITY OF TEXAS AT EL PASO/SOLAR ENERGY RESEARCH INSTITUTE,

Technical Report, 1985

Barcode

CSP Unique ID 190684105

Status

Electronic Resource

Call number

**Click on MARC view for more information on this report.**

Publication

SERI TR 253 2169; Report; June 1985.

Language

Library's review

ABSTRACT:
The present design methodology for the determination of wind loading on the various solar collectors has been reviewed and assessed. The total force coefficients of flat plates of aspect ratios 1.0 and 3.0, respectively, at various angles of attack obtained by using the guidelines of the
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ANSI A58.l-1982, have been compared v;ith those obtained by using the methodology of the ASCE Task Committee, 1961, and the experimental results of the full-scale test of heliostats -by Peglow. The turbulent energy spectra, currently employed in the building code, are compared with those of Kaimal et al., Lumley, and Ponofsky for wind velocities of 20.0 m/s and 40.24 m/s at an elevation of 9.15 m. The longitudal spectra of the building code overestimates the Kaimal spectra in the frequency range of 0.007 Hz -0.08 Hz and underestimates beyond the frequency of 0.08 Hz. The peak angles of attack, on the heliostat, stowed in horizontal position, due to turbulent vertical and lateral components of wind velocity, have been estimated by using Daniel 1s methodology for three wind velocities and compared with the value suggested by the code. The experimental results of a simple test in the laboratory indicate the feasibility of decreasing the drag forces of the flat plate by reducing the solidity ratio.
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