Fluxvector Splitting of the Inviscid Radiation Gas Dynamic Equations

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