1. IIA Institutional Repository
  2. Publications of Astronomical Society of India
  3. BASI Publications
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1802
Full metadata record
DC FieldValueLanguage
dc.contributor.authorBasu, S-
dc.contributor.authorChristensen-Dalsgaard, J-
dc.contributor.authorSchou, J-
dc.contributor.authorThompson, M. J-
dc.contributor.authorTomczyk, S-
dc.date.accessioned2007-09-19T06:46:01Z-
dc.date.available2007-09-19T06:46:01Z-
dc.date.issued1996-
dc.identifier.citationBASI, Vol.24 No. 2 pp. 147-150en
dc.identifier.urihttp://hdl.handle.net/2248/1802-
dc.description.abstractWe have used solar frequencies obtained form 1 year of observations with LOWL instrument to investigate the radial stratification of the Sun. Models which include the diffusion of helium and heavy elements below the solar convection zone are found to have a structure much closer to that of the Sun than models without diffusion. Also, models constructed with the Livermore(OPAL)equation of state seem to match the real Sun better than models constructed with the MHD equation of state. Finally, we find that an increase in the value of Z/X reduces the difference between models and Sun.en
dc.format.extent328939 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1996BASI...24..147Ben
dc.subjectSunen
dc.subjectInterior - Sunen
dc.subjectOscillations - Diffusionen
dc.titleSolar structure as revealed by 1 year LOWL dataen
dc.typeArticleen
Appears in Collections:BASI Publications

Files in This Item:
File Description SizeFormat 
Basu.pdf321.23 kBAdobe PDFThumbnail
View/Open
Show simple item record


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