Effects of thermal emission on Chandrasekhar's semi-infinite diffuse reflection problem

TL;DR

This paper extends Chandrasekhar's semi-infinite diffuse reflection model by incorporating thermal emission effects, resulting in modified scattering functions and reflected spectra that include temperature information, thus providing a more comprehensive atmospheric model.

Contribution

The authors generalize Chandrasekhar's model to include thermal emission, enhancing its accuracy for atmospheres with emission effects.

Findings

Scattering function is modified by B(T) with multiplicative factors.

Reflected spectra now include temperature information of the layer.

Model reduces to Chandrasekhar's original in absence of emission.

Abstract

Context: The analytical results of Chandrasekhar's semi-infinite diffuse reflection problem is crucial in the context of stellar or planetary atmosphere. However, the atmospheric emission effect was not taken into account in this model, and the solutions are applicable only for diffusely scattering atmosphere in absence of emission. Aim: We extend the model of semi-infinite diffuse reflection problem by including the effects of thermal emission B(T ), and present how this affects Chandrasekhar's analytical end results. Hence, we aim to generalize Chandrasekhar's model to provide a complete picture of this problem. Method: We use Invariance Principle Method to find the radiative transfer equation accurate for diffuse reflection in presence of B(T ). Then we derive the modified scattering function S(${\mu},{\phi}; {\mu}_0 , {\phi}_0$ ) for different kind of phase functions. Results: We find that, the scattering function S(${\mu}, {\phi}; {\mu}_0 , {\phi}_0$ ) as well as diffusely reflected specific intensity $I(0, {\mu}; {\mu}_0 )$ for different phase functions are modified due to the emission $B(T)$ from layer ${\tau} = 0$. In both cases, B(T) is added to the results of only scattering case derived by Chandrasekhar, with some multiplicative factors. Thus the diffusely reflected spectra will be enriched and carries the temperature information of ${\tau} = 0$ layer. As the effects are additive in nature, hence our model reduces to the sub-case of Chandrasekhar's scattering model in case of $B(T) = 0$. We conclude that our generalized model provides more accurate results due to the inclusion of the thermal emission effect in Chandrasekhar's semi-infinite atmosphere problem.