Abstract
This study makes an analysis of the radiation heat transfer in a turbulent non-premixed methane–air cylindrical combustion chamber. The highly complex dependence of the radiative properties with the wavenumber spectrum is modeled with the weighted-sum-of-gray-gas (WSGG), making use of the classical correlations of Smith et al. (J Heat Transfer 104:602–608, 1982) and of the more recently in obtained correlations of Dorigon et al. (IJHMT 64:863–873, 2013), based on HITEMP2010. The reaction rates were considered as the minimum values between the Arrhenius and Eddy Break-Up rates. A two-step global reaction mechanism was used, and turbulence modeling was considered via standard k–ε model. The source terms of the energy equation consisted of the energy involved in the reaction rates and radiation exchanges. The discrete ordinates method (DOM) was employed to solve the radiative transfer equation (RTE). The results show that the temperature, the radiative heat source, and the wall heat flux can be importantly affected by the WSGG correlations, while their influence on the species concentrations tends to be negligible. Numerical results considering the WSGG model with the new correlations were closer to experimental data presented in the literature.
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Abbreviations
- a j (T) :
-
Emission weighted factor (WSGG), dimensionless
- b j :
-
Polynomial coefficients of the WSGG model, units can vary
- c :
-
Each reaction on mechanism, dimensionless
- c p,α :
-
Specific heat, J/(kg K)
- C 1,ε , C 2,ε :
-
Constants of the turbulence model, dimensionless
- C μ :
-
Constant of the turbulence model, dimensionless
- CH4 :
-
Methane
- CO:
-
Carbon monoxide
- CO2 :
-
Carbon dioxide
- f rad :
-
Radiant fraction, dimensionless
- h :
-
Specific enthalpy, J/kg
- \( h_{\alpha }^{0} \) :
-
Formation enthalpy of species α, J/kg
- H2O:
-
Water vapor
- I :
-
Total radiative intensity, W/m²
- I η :
-
Spectral radiative intensity, W/(m² m−1)
- K :
-
Turbulent kinetic energy, m²/s²
- k j :
-
Absorption coefficient for the j-th gray gas for WSGG model, m−1
- k p,j :
-
Pressure absorption coefficient for the j-th gray gas for WSGG model, m−1 atm−1
- \( \bar{M}\bar{M}_{\alpha } \) :
-
Molar mass, kg/kmol
- n :
-
Vector normal to the surface element, dimensionless
- N G :
-
Number of gray gases (WSGG), dimensionless
- N2 :
-
Nitrogen
- O2 :
-
Oxygen
- p :
-
Pressure, Pa
- \( p_{{{\text{H}}_{ 2} {\text{o}}}} /p_{{{\text{CO}}_{ 2} }} \) :
-
Ratio of H2O and CO2 partial pressures, dimensionless
- p* :
-
Modified pressure, Pa
- Pr t , Sc t :
-
Turbulent Prandtl and Schmidt numbers, dimensionless
- \( {\mathbf{q}}_{r} \) :
-
Radiative heat flux, W/m²
- r :
-
Radial coordinate, m
- \( \bar{R} \) :
-
Universal gas constant, J/(kmol K)
- R α :
-
Volumetric rate of formation or destruction of α, kg/(m³ s)
- s :
-
Distance traveled by the radiation intensity, m
- s :
-
Vector in the direction of the radiation intensity, dimensionless
- S rad :
-
Radiative heat source, W/m³
- S ϕ :
-
Source term for ϕ, W/m³
- T :
-
Temperature, K
- u :
-
Axial velocity, m/s
- v :
-
Radial velocity, m/s
- w :
-
Angular velocity, m/s
- y α :
-
Mass fraction, kgα/kgmix
- z :
-
Axial coordinate, m
- ε :
-
Dissipation rate of k, m²/s³
- ε w :
-
Wall emissivity, dimensionless
- ϕ :
-
Generic variable, units can vary
- φ :
-
Angular coordinate, rad
- Γ ϕ :
-
Diffusive coefficient for ϕ, N s/m²
- κ η :
-
Spectral absorption coefficient, m−1
- μ :
-
Viscosity, N s/m²
- μ t :
-
Turbulent viscosity, N s/m²
- μ, ς, ξ :
-
Discrete ordinates method directions
- ρ :
-
Density, kg/m³
- σ k , σ ε :
-
Prandtl numbers for k and ε, dimensionless
- Ω :
-
Solid angle, sr
- b :
-
Blackbody
- Dorigon:
-
WSGG model coefficients from Dorigon et al. [6]
- j :
-
Each gray gas of the WSGG model
- rad:
-
Radiation
- ref:
-
Reference
- Smith:
-
WSGG model coefficients from Smith et al. [25]
- w :
-
Wall
- α :
-
Each chemical species
- η :
-
Wavenumber, m−1
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Acknowledgments
Authors FHRF and HAV thank CNPq (Brazil) for research Grants 304728/2010-1, 473899/2011-6 and 470325/2011-9, 303823/2012-7, respectively.
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Technical Editor: Luis Fernando Figueira da Silva.
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Centeno, F.R., Cassol, F., Vielmo, H.A. et al. Comparison of different WSGG correlations in the computation of thermal radiation in a 2D axisymmetric turbulent non-premixed methane–air flame. J Braz. Soc. Mech. Sci. Eng. 35, 419–430 (2013). https://doi.org/10.1007/s40430-013-0040-z
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DOI: https://doi.org/10.1007/s40430-013-0040-z