Detalles de publicación
PP 020032
The Stellar Atmosphere Physical System II An Operative Sequential Algorithm to Solve the Stellar Atmosphere Problem
Instituto de Astrofísica de Canarias, Departamento de Astrofísica Universidad de La Laguna & INAF-Osservatorio Astronomico di Trieste (Italy)
In this paper, the second and the last of the series, we present a sequential algorithm to solve the stellar atmosphere problem that may serve as a paradigm for the solution of more general non-linear and non-local problems.The Iteration Factors (IF) Method is applied to achieve a solution of the radiativetransfer equations, consistent with the radiative equilibrium constraint.
