Please use this identifier to cite or link to this item: http://nopr.niscpr.res.in/handle/123456789/3832
Full metadata record
DC FieldValueLanguage
dc.contributor.authorShanker, B-
dc.contributor.authorBabu, A Benerji-
dc.date.accessioned2009-04-15T04:40:29Z-
dc.date.available2009-04-15T04:40:29Z-
dc.date.issued2006-04-
dc.identifier.issn0367-8393-
dc.identifier.urihttp://hdl.handle.net/123456789/3832-
dc.description84-89en_US
dc.description.abstractThe linear stability of convection due to oblique magnetic field in the penumbral region of sunspot has been investigated. We have obtained the values of Takens-Bogdanov bifurcation points and co-dimension two-bifurcation points by plotting graphs of neutral curves corresponding to stationary and oscillatory convection for different values of physical parameters relevant to convection in the penumbral region of sunspot.en_US
dc.language.isoen_USen_US
dc.publisherCSIRen_US
dc.sourceIJRSP Vol.35(2) [April 2006]en_US
dc.subjectConvectionen_US
dc.subjectPenumbraen_US
dc.subjectBifurcation pointsen_US
dc.titleConvection due to oblique magnetic field in the penumbral region of sunspoten_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.35(2) [April 2006]

Files in This Item:
File Description SizeFormat 
IJRSP 35(2) 84-89.pdf295.03 kBAdobe PDFView/Open


Items in NOPR are protected by copyright, with all rights reserved, unless otherwise indicated.