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2019•Serbian Astronomical JournalOpen access

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

L. Crivellari

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Abstract

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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What this paper is about

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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Available abstract

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.

Key concepts: Radiative transfer, Physics, Atmosphere (unit), Stellar atmosphere, Constraint (computer-aided design), Radiative equilibrium, Algorithm, Series (stratigraphy)

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