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On the Dependence of the Two-Level Source Function on its Own Radiation Field

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1973

Year

Abstract

The consequences of the universally made assumption that the stimulated emission profile is identical to the absorption profile are quantitatively investigated for a two-level atom with Doppler redistribution. The non-linear terms arising in the source function are evaluated iteratively. We find that the magnitude of the effects are governed by ζ = (exp ( hv / kT ) − 1) −1 and are probably completely negligible for visible and UV solar lines. For ζ = 2 effects of ∼5 per cent are encountered. Larger ζ 's lead to numerical instabilities in the method of solution used.