Flow of Gas along a Magnetic field with Time-Dependent Geometry

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/372

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DC Field	Value	Language
dc.contributor.author	Hasan, S. S	-
dc.contributor.author	Venkatakrishnan, P	-
dc.date.accessioned	2005-03-02T06:31:59Z	-
dc.date.available	2005-03-02T06:31:59Z	-
dc.date.issued	1980	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 3, pp. 6-16	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/372	-
dc.description.abstract	The flow of gas along a magnetic field with time dependent geometry has been studied. It is seen that the velocity of the flow in the direction of the magnetic field depends both on the magnitude of the velocity of flow perpendicular to the field as well as on its spatial variation. Further, the nature of the flow is not very senstive to the choice of base temperature and polytropic index. The application of this study to magnetofluid dynamic flow on the Sun is discussed.	en
dc.format.extent	266033 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Fluid dynamics	en
dc.subject	One Dimensional unsteady flow	en
dc.subject	Astrophysics	en
dc.subject	Sun	en
dc.subject	Magnetofluid Dynamics	en
dc.title	Flow of Gas along a Magnetic field with Time-Dependent Geometry	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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