Detalles de publicación

PP 020032

The Stellar Atmosphere Physical System II An Operative Sequential Algorithm to Solve the Stellar Atmosphere Problem

L. Crivellari
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.

 
Aceptado para publicación en | Enviado el 2020-02-04 | Proyecto P309808