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/2248/2036
Full metadata record
DC FieldValueLanguage
dc.contributor.authorBasu, S-
dc.date.accessioned2008-02-23T07:41:01Z-
dc.date.available2008-02-23T07:41:01Z-
dc.date.issued2000-
dc.identifier.citationBASI, Vol. 28, No. 1, pp. 63 - 69en
dc.identifier.urihttp://hdl.handle.net/2248/2036-
dc.description.abstractThe "Seismic Sun" is a model of the Sun constructed using helioseismological deductions about the Sun. The seismic Sun is very similar to a standard solar model which incorporates gravitational settling of helium and heavy elements. The main discrepancy is just below the base of the convection zone and can be attributed to the lack of mixing in standard solar models.en
dc.format.extent593434 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000BASI...28...63Ben
dc.subjectSun: Oscillationsen
dc.subjectSun: Interioren
dc.titleThe seismic sunen
dc.typeArticleen
Appears in Collections:BASI Publications

Files in This Item:
File Description SizeFormat 
Basu.pdf579.53 kBAdobe PDFThumbnail
View/Open
Show simple item record


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