Radiation From a Directional Source: Beam Divergence in Solar Simulators

[+] Author and Article Information
R. P. Bobco

Hughes Aircraft Co., Space Systems Division, Los Angeles, Calif.

J. Eng. Power 87(3), 259-269 (Jul 01, 1965) (11 pages) doi:10.1115/1.3678241 History: Received March 24, 1964; Online January 10, 2012


The analysis of thermal phenomena associated with radiation from sources which are imperfectly collimated is presented in a form convenient for engineering calculations. The analysis is developed in terms of beam divergence and directional intensity and applied to an hypothetical solar simulation system. Two different intensity distributions are postulated and expressions are derived for solar constants and solar shape factors. The concept of shadowing is discussed and a procedure is described for calculating both local and mean solar shape factors in penumbral regions. A simple L-shaped configuration is analyzed to illustrate the procedures and to examine the influence of beam divergence on equilibrium temperatures. Results are presented for both diffuse and specular surfaces, and several values of α*/ε.

Copyright © 1965 by ASME
Your Session has timed out. Please sign back in to continue.





Some tools below are only available to our subscribers or users with an online account.

Related Content

Customize your page view by dragging and repositioning the boxes below.

Related Journal Articles
Related eBook Content
Topic Collections

Sorry! You do not have access to this content. For assistance or to subscribe, please contact us:

  • TELEPHONE: 1-800-843-2763 (Toll-free in the USA)
  • EMAIL: asmedigitalcollection@asme.org
Sign In