New approach for inclusion of the effect of gravity in magnetohydrostatic equilibrium in solar coronal arcades

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1460

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DC Field	Value	Language
dc.contributor.author	Prasad, L	-
dc.contributor.author	Chandra, S	-
dc.date.accessioned	2007-03-21T06:57:32Z	-
dc.date.available	2007-03-21T06:57:32Z	-
dc.date.issued	1992	-
dc.identifier.citation	BASI, Vol. 20, pp. 65-73	en
dc.identifier.uri	http://hdl.handle.net/2248/1460	-
dc.description.abstract	The study presents a novel approach for the inclusion of the effect of gravity in the magnetohydrostatic equilibrium in coronal arcades, in which the magnetic lines of force are unaffected whereas the pressure isobars are distorted owing to the inclusion of the effect of gravity. In the earlier approach, it was an essential requirement to represent plasma by an ideal gas, whereas the present approach remains unaffected whether plasma is represented by an ideal gas or not	en
dc.format.extent	596445 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Solar Corona	en
dc.title	New approach for inclusion of the effect of gravity in magnetohydrostatic equilibrium in solar coronal arcades	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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