An implicit integral method to solve selected radiative transfer problems. 3: Factorization versus linearization
In view of more general applications, we have developed a new approach to render explicit the temperature both in the source function of the radiative transfer equation and in the constraint of radiative equilibrium. This is a necessary step in the iterative temperature correction when computing stellar atmosphere models. Our method consists of a
Crivellan, L. et al.
Fecha de publicación:
6
1994