Abstract
In the present work, the full spectrum k-distribution method (FSK) has been adopted to calculate the radiative transfer in the presence of participating gaseous medium within an enclosure. The radiative properties of the medium is obtained from the HITEMP-2010 database. Further, the radiative properties have been assembled into a monotonically increasing function using the FSK. Moreover, a look-up table has been developed for these properties at different thermodynamic states and a multi-dimensional linear interpolation technique for unavailable thermodynamic states of gases. Furthermore, the FSK method is extended for mixture of gases using different mixing models such as superposition, multiplication and hybrid models. The radiation transfer equation (RTE) is solved by finite angle method to calculate the wall heat fluxes and the divergence of radiative heat flux for various test cases in the categories of homogeneous and non-homogeneous medium having different conditions of temperature and mole-fraction. The multiplication mixing model produces most accurate results among the mixture models used here. The results obtained from FSK has been validated against benchmark solution of line by line method (LBL). The FSK method has been also successfully applied to non-homogeneous gaseous medium for single gas or mixture of gases with almost LBL accuracy at extremely less computational cost.
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Abbreviations
- G :
-
Irradiation
- \(I_\eta \) :
-
Spectral intensity
- \(I_{b\eta }\) :
-
Planck function
- N :
-
Number density of species
- \(N_g\) :
-
Number of participating gases
- Q :
-
Partition function
- \(S_{if}\) :
-
Line intensity
- \(T_{ref}\) :
-
Reference temperature
- a :
-
Stretching function
- f :
-
Fractional Planck function
- g :
-
cumulative k-distribution
- k :
-
re-ordered absorption coefficient
- \(k_{if}\) :
-
Absorption crossection
- p :
-
Number of quadrature points
- \(p_{self}\) :
-
Self pressure of gas
- q :
-
Radiative heat flux
- s :
-
Direction vector
- w :
-
weight for quadrature integration
- \(\beta _\eta \) :
-
Spectral extinction coefficient
- \(\delta \) :
-
Line shift
- \(\epsilon _{w\eta }\) :
-
Spectral emissivity of the wall
- \(\eta \) :
-
Wavenumber
- \(\gamma \) :
-
Half width at half maximum
- \(\gamma _{air}\) :
-
Air broadened half width
- \(\gamma _{self}\) :
-
Self broadened half width
- \(\kappa _\eta \) :
-
Spectral absorption coefficient
- \(\nabla \cdot q\) :
-
Divergence of radiative heat flux
- \(\nu _{if}\) :
-
Vacuum wavenumber
- \(\Omega \) :
-
Solid angle
- \(\Phi _\eta \) :
-
Spectral scattering phase function
- \(\sigma _{s\eta }\) :
-
Spectral scattering coefficient
- \(\eta \) :
-
Wavenumber
- g :
-
gas
- if :
-
transition from upper state f to lower state i
- ref :
-
reference
- w :
-
wall
- air:
-
air
- self:
-
self
- \(P_N\) :
-
Spherical harmonics method
- ADF:
-
Absorption distribution function
- CDSD:
-
Carbon-dioxide spectroscopic database
- DOM:
-
Discrete ordinate method
- DTM:
-
Discrete transfer model
- FSK:
-
Full spectrum k-distribution method
- FVM:
-
Finite volume method
- HITEMP:
-
High temperature spectroscopic absorption parameter
- HITRAN:
-
High resolution transmission spectroscopic molecular absorption database
- HMM:
-
Hybrid mixing model
- HWHM:
-
Half width at half maximum
- LBL:
-
Line-by-line
- MMM:
-
Multiplication mixing model
- RTE:
-
Radiation transfer equation
- SAM:
-
Spectral addition method
- SLW:
-
Spectral line weighted sum-of-gray gases model
- SMM:
-
Superposition mixing model
- WSGG:
-
Weighted sum-of-gray gas model
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Khemani, K., Parvatikar, S. & Kumar, P. Radiative heat transfer calculations using full spectrum k-distribution method for benchmark test cases. Sādhanā 48, 3 (2023). https://doi.org/10.1007/s12046-022-02059-y
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DOI: https://doi.org/10.1007/s12046-022-02059-y