The stellar atmosphere physical system II. An operative sequential algorithm to solve the stellar atmosphere problem

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 r...

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Main Author: Crivellari Lucio
Format: Article
Language:English
Published: Astronomical Observatory, Department of Astronomy, Belgrade 2019-01-01
Series:Serbian Astronomical Journal
Subjects:
Online Access:http://www.doiserbia.nb.rs/img/doi/1450-698X/2019/1450-698X1900001C.pdf
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author Crivellari Lucio
author_facet Crivellari Lucio
author_sort Crivellari Lucio
collection DOAJ
description 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 radiative transfer equations, consistent with the radiative equilibrium constraint.
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spelling doaj.art-1a899f03852c4e0d823f7e30ed1837882022-12-21T22:33:39ZengAstronomical Observatory, Department of Astronomy, BelgradeSerbian Astronomical Journal1450-698X1820-92892019-01-01201919811110.2298/SAJ190215001C1450-698X1900001CThe stellar atmosphere physical system II. An operative sequential algorithm to solve the stellar atmosphere problemCrivellari Lucio0Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain + Departamento de Astrofísica, Universidad de La Laguna, Tenerife, Spain + INAF - Osservatorio Astronomico di Trieste, Trieste, ItalyIn 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 radiative transfer equations, consistent with the radiative equilibrium constraint.http://www.doiserbia.nb.rs/img/doi/1450-698X/2019/1450-698X1900001C.pdfstars: atmospheresmethods: numericalradiative transfer
spellingShingle Crivellari Lucio
The stellar atmosphere physical system II. An operative sequential algorithm to solve the stellar atmosphere problem
Serbian Astronomical Journal
stars: atmospheres
methods: numerical
radiative transfer
title The stellar atmosphere physical system II. An operative sequential algorithm to solve the stellar atmosphere problem
title_full The stellar atmosphere physical system II. An operative sequential algorithm to solve the stellar atmosphere problem
title_fullStr The stellar atmosphere physical system II. An operative sequential algorithm to solve the stellar atmosphere problem
title_full_unstemmed The stellar atmosphere physical system II. An operative sequential algorithm to solve the stellar atmosphere problem
title_short The stellar atmosphere physical system II. An operative sequential algorithm to solve the stellar atmosphere problem
title_sort stellar atmosphere physical system ii an operative sequential algorithm to solve the stellar atmosphere problem
topic stars: atmospheres
methods: numerical
radiative transfer
url http://www.doiserbia.nb.rs/img/doi/1450-698X/2019/1450-698X1900001C.pdf
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