Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4966
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dc.contributor.authorAnusha, L. S-
dc.contributor.authorNagendra, K. N-
dc.date.accessioned2010-01-08T16:28:27Z-
dc.date.available2010-01-08T16:28:27Z-
dc.date.issued2009-
dc.identifier.citationMemorie della Societa Astronomica Italiana, Vol. 80, pp. 631 - 633en
dc.identifier.issn1824-016X-
dc.identifier.urihttp://hdl.handle.net/2248/4966-
dc.descriptionOpen Access-
dc.description.abstractAn efficient numerical method called the Preconditioned Bi-Conjugate Gradient (Pre-BiCG) method is presented for the solution of radiative transfer equation in spherical geometry. A variant of this method called Stabilized Preconditioned Bi-Conjugate Gradient (Pre-BiCG-STAB) is also presented. These methods are based on projections on the subspaces of the n dimensional Euclidean space mathbb {R}n called Krylov subspaces. The methods are shown to be faster in terms of convergence rate compared to the contemporary iterative methods such as Jacobi, Gauss-Seidel and Successive Over Relaxation (SOR).en
dc.language.isoenen
dc.publisherSocieta Astronomica Italianaen
dc.relation.urihttp://sait.oat.ts.astro.it/MSAIt800309/index.htmlen
dc.rights© Societa Astronomica Italianaen
dc.subjectLine: Formationen
dc.subjectNumerical Radiative Transferen
dc.subjectMethods: Techniquesen
dc.titleProjection methods for line radiative transfer in spherical mediaen
dc.typeArticleen
Appears in Collections:IIAP Publications

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