Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1460
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dc.contributor.authorPrasad, L-
dc.contributor.authorChandra, S-
dc.date.accessioned2007-03-21T06:57:32Z-
dc.date.available2007-03-21T06:57:32Z-
dc.date.issued1992-
dc.identifier.citationBASI, Vol. 20, pp. 65-73en
dc.identifier.urihttp://hdl.handle.net/2248/1460-
dc.description.abstractThe 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 noten
dc.format.extent596445 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectSolar Coronaen
dc.titleNew approach for inclusion of the effect of gravity in magnetohydrostatic equilibrium in solar coronal arcadesen
dc.typeArticleen
Appears in Collections:BASI Publications

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