Astronomy & Astrophysics

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Issue		A&A Volume 411, Number 2, November IV 2003
Page(s)		221 - 227
Section		Formation and evolution of planetary systems
DOI		10.1051/0004-6361:20031240

A&A 411, 221-227 (2003)
DOI: 10.1051/0004-6361:20031240

On the accuracy of the ALI method for solving the radiative transfer equation

L. Chevallier¹, F. Paletou² and B. Rutily¹

¹ Centre de Recherche Astronomique de Lyon, UMR 5574 du CNRS, Observatoire de Lyon, 9 avenue Charles André, 69561 Saint-Genis-Laval Cedex, France
e-mail: rutily@obs.univ-lyon1.fr
² Observatoire de la Côte d'Azur, Département G. D. Cassini, UMR 6529 du CNRS, BP 4229, 06304 Nice Cedex 4, France
e-mail: fpaletou@mail.ast.obs-mip.fr

(Received 25 April 2003 / Accepted 30 July 2003)

Abstract
We solve the integral equation describing the propagation of light in an isothermal plane-parallel atmosphere of optical thickness $\tau^*$ , adopting a uniform thermalization parameter $\epsilon$ . The solution given by the ALI method, widely used in the field of stellar atmosphere modelling, is compared to the exact solution. Graphs are given that illustrate the accuracy of the ALI solution as a function of the parameters $\epsilon$ , $\tau^*$ and optical depth variable $\tau$ .

Key words: radiative transfer -- methods: numerical -- stars: atmospheres

Offprint request: L. Chevallier, loic.chevallier@obs.univ-lyon1.fr

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