Fluxvector Splitting of the Inviscid Radiation Gas Dynamic Equations

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/378

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DC Field	Value	Language
dc.contributor.author	Peraiah, A	-
dc.date.accessioned	2005-03-04T04:30:13Z	-
dc.date.available	2005-03-04T04:30:13Z	-
dc.date.issued	1980	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 3, pp. 49-56	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/378	-
dc.description.abstract	We have analysed various schemes for the iterative simultaneous solution of the inviscid gas dynamic equations. We have considered the problem from the point of view of the stellar atmospheres. The difference between conservative and quasiconservative systems has been analysed by using the flux vector splitting process. The radiation pressure in the atmosphere (due to continuum and resonance lines) has been included in flux vector splitting analysis to obtain best difference schemes.	en
dc.format.extent	129883 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Fluxvector Splitting	en
dc.subject	Radiation Gas Dynamics	en
dc.title	Fluxvector Splitting of the Inviscid Radiation Gas Dynamic Equations	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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