Hostname: page-component-cd9895bd7-dk4vv Total loading time: 0 Render date: 2024-12-28T04:22:07.239Z Has data issue: false hasContentIssue false

Radiative transfer effects in natural convection above fires

Published online by Cambridge University Press:  28 March 2006

M. P. Murgai
Affiliation:
Harvard University, Cambridge, Massachusetts

Abstract

This paper describes the results of examining the influence of radiative heat transfer on turbulent natural convection above fires in an atmosphere of constant potential temperature, under both the ‘opaque’ and ‘transparent’ approximations. It turns out that on the basis of the over-all approximations introduced in this investigation, the former case reduces to that of no radiative transfer. For the latter case, the initial fire size, the energy release rate (initial temperature difference) and the absorption coefficient have been regarded as independent parameters. The solution curves presented cover a range over which these parameters are expected to vary in practice.

Type
Research Article
Copyright
© 1962 Cambridge University Press

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Chandrasekhar, S. 1939 Stellar Structure. University of Chicago Press.
Hottel, H. C. & Mangelsdorf, H. G. 1935 Trans. Amer. Inst. Chem. Engrs, 31, 517.
Hottel, H. C. & Smith, V. C. 1935 Trans. Amer. Soc. Mech. Engrs, 57, 463.
Kourganoff, V. 1952 Basic Methods in Transfer Problems. Oxford University Press.
Murgai, M. P. & Emmons, H. W. 1960 J. Fluid Mech. 8, 611.