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Volumn 1, Issue 2, 2009, Pages 207-230

Higher-order spherical harmonics to model radiation in direct numerical simulation of turbulent reacting flows

Author keywords

[No Author keywords available]

Indexed keywords

ABSORPTION COEFFICIENTS; COMPUTATIONAL RESOURCES; DISCRETE ORDINATES METHOD; FIRST ORDER PARTIAL DIFFERENTIAL EQUATIONS; GENERAL BOUNDARY CONDITIONS; GRAY GAS; HIGHER ORDER; HIGHER-ORDER APPROXIMATION; HYDROCARBON-AIR COMBUSTION; INTENSITY CORRELATION; MEAN ABSORPTION; MOMENT METHODS; NONLINEAR COUPLING; NUMERICAL SOLUTION; OPTICAL THICKNESS; PHOTON MONTE CARLO METHOD; PLANCK FUNCTION; RADIATION PROPERTIES; RADIATIVE INTENSITY; RADIATIVE PROCESS; RADIATIVE TRANSFER EQUATIONS; SECOND-ORDER PARTIAL DIFFERENTIAL EQUATION; SELF-CORRELATION; SOLUTION METHODS; SPECIES CONCENTRATION; SPECTRAL METHODS; SPHERICAL HARMONICS; SPHERICAL HARMONICS METHOD; STATISTICAL NOISE; SUCCESSIVE ELIMINATION; THIRD-ORDER; THREE DIMENSIONAL GEOMETRY; TURBULENCE-RADIATION INTERACTION; TURBULENT REACTING FLOWS; VARIABLE PROPERTY;

EID: 75549083556     PISSN: 19402503     EISSN: 19402554     Source Type: Journal    
DOI: 10.1615/ComputThermalScien.v1.i2.60     Document Type: Article
Times cited : (18)

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