The Astrophysical Journal · 1981 · 112 citations · 0 references
Natural SciencesAstronomyAtmospheric RadiationAtmospheric ThermodynamicsRadiation TransportNumerical AnalysisNumerical Methods For Differential EquationsPerturbation TheoryRadiative EquilibriumRadiative ProcessesRadiative TransferConvergenceEddington ApproximationRadiative Transfer ApproximationRadiative Transfer EquationsRadiative Transfer ModelingRadiative Transfer TheoryRadiative Transport TheorySource Function
An approximate analytical method and an exact numerical method for solving non-LTE problems are presented. The analytical method relies on concepts of radiative transfer theory such as the core-saturation approximation, the Eddington-Barbier relation, and the upper boundary condition, to derive a simple first-order differential equation for the line source function. The more efficient technique is developed using a linear test function and a one-point quadrature relation between the specific intensity and the source function. A 1% accuracy in the line source function can be obtained after four iterations, with a very rapid convergence and no evidence of numerical instabilities.