Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12188/1555
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dc.contributor.authorKuzmanovska, Olgica; Atanackovic, Olga; Faurobert, Marianneen_US
dc.date.accessioned2019-03-07T14:29:26Z-
dc.date.available2019-03-07T14:29:26Z-
dc.date.issued2019-
dc.identifier.urihttp://hdl.handle.net/20.500.12188/1555-
dc.description.abstractThe Forth-and-Back Implicit Lambda Iteration (FBILI) is efficient Gauss-Seidel-type iterative scheme developed by Atanackovic-Vukmanovic et al. [1] for a solution of non-LTE radiative transfer (RT) problems of spectral line formation in stellar atmospheres. In [2] it was more explicitly implemented on non-linear line transfer in multi-level atomic models in 1D geometry, providing high convergence rate to the exact solution with no use of additional acceleration techniques. Here, we apply FBILI on a standard benchmark problem of CaII line formation in the solar atmosphere using the VALCH atmospheric model. Additionally we compare its accuracy with the well known code MULTI.en_US
dc.description.sponsorshipInstitute of Physics, Faculty of Natural Sciences and Mathematics, Skopje, Republic of Macedoniaen_US
dc.language.isoenen_US
dc.publisherSociety of Physicists of Macedoniaen_US
dc.relationMethods of solution for radiative transfer problems in stellar atmospheresen_US
dc.subjectradiative transfer, methods: numerical, stars, atmospheresen_US
dc.titleApplication of FBILI method for multi-level line transferen_US
dc.typeProceeding articleen_US
dc.relation.conference12th Conference of the Society of Physicists of Macedoniaen_US
item.grantfulltextnone-
item.fulltextNo Fulltext-
Appears in Collections:Faculty of Natural Sciences and Mathematics: Conference papers
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