Solution of a radiative transfer equation with Pomraning Phase function and a linear source in a semi-infinite medium

摘要

The equation of radiative transfer with Pomraning phase function and a linear source in a plane parallel semi-infinite atmosphere with axial symmetry has been solved by Laplace transform and Wiener-Hopf technique We have determined the emergent intensity in terms of Chandrasekhar's H-function and the intensity at any optical depth by inversion.