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/2248/3511
Full metadata record
DC FieldValueLanguage
dc.contributor.authorTripathy, S. C-
dc.contributor.authorChristensen-Dalsgaard, J-
dc.date.accessioned2008-09-09T12:58:18Z-
dc.date.available2008-09-09T12:58:18Z-
dc.date.issued1998-
dc.identifier.citationBASI, Vol. 26, pp. 163 - 165en
dc.identifier.urihttp://hdl.handle.net/2248/3511-
dc.description.abstractWe investigate the effect of localized opacity modifications on the sound-speed profile of solar models. The sound-speed difference between the Sun and a solar model is used to deduce the opacity correction that would be required to bring the model into agreement with the Sun. We test this procedure on artificial data for a pair of solar models and apply it to the solar sound speed as inferred from inversion of LOWL observed frequencies. We show that a solar model constructed with the appropriately modified opacity has a sound-speed profile very similar to that of the Sun.en
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1998BASI...26..163Ten
dc.subjectHelioseismologyen
dc.subjectSolar oscillationen
dc.subjectOpacityen
dc.titleTesting the helioseismic determination of opacity correctionsen
dc.typeArticleen
Appears in Collections:BASI Publications

Files in This Item:
File Description SizeFormat 
tripathy.pdf147.95 kBAdobe PDFThumbnail
View/Open
Show simple item record


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