RESEARCH ARTICLE

Nongray radiation from gas and soot mixtures in planar plates based on statistical narrow-band spectral model

  • Huaqiang CHU 1 ,
  • Qiang CHENG 1 ,
  • Huaichun ZHOU , 1 ,
  • Fengshan LIU 2
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  • 1. State Key Laboratory of Coal Combustion, Huazhong University of Science and Technology, Wuhan 430074, China
  • 2. Institute for Chemical Process and Environmental Technology, National Research Council, Ottawa, Ont, K1A 0R6 Canada

Received date: 30 Apr 2010

Accepted date: 15 Jul 2010

Published date: 05 Jun 2011

Copyright

2014 Higher Education Press and Springer-Verlag Berlin Heidelberg

Abstract

The nongray behavior of combustion products plays an important role in various areas of engineering. Based on the statistical narrow-band (SNB) spectral model with an exponential-tailed inverse intensity distribution and the ray-tracing method, a comprehensive investigation of the influence of soot on nongray radiation from mixtures containing H2O/N2+soot, CO2/N2+soot, or H2O/CO2/N2+soot was conducted in this paper. In combustion applications, radiation transfer is significantly enhanced by soot due to its spectrally continuous emission. The effect of soot volume fraction up to 1×10-6 on the source term, the narrow-band radiation intensities along a line-of-sight, and the net wall heat fluxes were investigated for a wide range of temperature. The effect of soot was significant and became increasingly drastic with the increase of soot loading.

Cite this article

Huaqiang CHU , Qiang CHENG , Huaichun ZHOU , Fengshan LIU . Nongray radiation from gas and soot mixtures in planar plates based on statistical narrow-band spectral model[J]. Frontiers in Energy, 2011 , 5(2) : 149 -158 . DOI: 10.1007/s11708-010-0124-8

Acknowledgements

This work was supported by the National Natural Science Foundation of China (Grant Nos. 50636010, 50906027).
Notations
fspecies molar fraction
Iradiation intensity/(W·m-2·sr-1)
Ivspectral radiation intensity/(W·m-2·sr-1·cm-1)
kvmean line-intensity to spacing ratio/(cm-1·atm-1)
k¯vequivalent mean line-intensity to spacing ratio/(cm-1·atm-1)
Lseparation distance between parallel walls/m
ppressure/atm
qheat flux density/(kW·m-2)
s,sposition variables/m
xCartesian coordinates/m
β¯vmean line-width to spacing ratio
γ¯vmean half-width of an absorption line/cm-1
δ¯vequivalent line spacing/cm-1
Δvwavenumber interval/cm-1
νwavenumber/cm-1
μdirection cosines
τνspectral transmittance
Subscripts
bblackbody
ispatial discretization (along a line-of-sight) index
nangular discretization index
wwall
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