EAS Publications Series
Volume 5, 2002Radiative Transfer and Hydrodynamics in Astrophysics
|Page(s)||31 - 31|
|Published online||25 September 2002|
Ph. Stee (ed)
EAS Publications Series, 5 (2002) 31
SOME ITERATIVE METHODS FOR RADIATIVE TRANSFER PROBLEMS
Institut d'Astrophysique, CNRS, 98bis boulevard Arago, 75014 Paris, France
2 Observatorio Astronomico di Trieste, and Instituto de AstrofÃsica de Canarias, Via Lactea s/n, 38200 La Laguna (Tenerife), Spain
In the mathematical computation of many physical problems we have to work with the numerical solution of non-linear problems. Even in case that a direct solution does in principle exist, its feasibility is however actually restricted to a very limited number of instances. Therefore, in this study we will disregard this possibility. Consequently, we assume that an iterative procedure shall be necessary in order to tackle, in practice, all kind of non-linear problems.
© EAS, EDP Sciences, 2002
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.