Discrete Space Theory of Radiative Transfer: Application

Srinivasa Rao, M

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dc.contributor.author	Srinivasa Rao, M
dc.date.accessioned	2010-08-20T12:47:36Z
dc.date.available	2010-08-20T12:47:36Z
dc.date.issued	2010
dc.identifier.citation	Chaudhuri, R. K., Mekkaden, M. V., Raveendran, A. V & Narayanan, A. S., eds., Recent Advances In Spectroscopy: Theoretical, Astrophysical And Experimental Perspectives, Proceedings of the International Conference on Recent Advances in Spectroscopy - Theoretical, Astrophysical and Experimental Perspectives, Jan 28-31, 2009, Indian Institute of Astrophysics, Kodaikanal Observatory, Bangalore, India, pp. 155-161	en
dc.identifier.uri	http://hdl.handle.net/2248/5228
dc.description	The original publication is available at springerlink.com	en
dc.description.abstract	The method of obtaining the solution of radiative transfer equation using discrete space theory (DST) is described with (1) interaction principle for different geometries (2) star product (3) calculation of radiation field at internal points. Some of the important steps to obtain the solution of radiative transfer equation in spherical symmetry are also mentioned. Applications of DST are discussed with their results in two cases (a) study of reflection effect in close binary systems and (b) to compute KI 769.9 nm emission line profiles from N-type stars.	en
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.ispartofseries	Astrophysics and Space Science Proceedings;
dc.relation.uri	http://www.springerlink.com/content/l788177w7l41183p/	en
dc.rights	© Springer	en
dc.subject	Radiative transfer	en
dc.subject	Discrete space theory	en
dc.subject	Close binaries	en
dc.subject	Circumstellar envelope	en
dc.title	Discrete Space Theory of Radiative Transfer: Application	en
dc.type	Article	en