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/2248/2038
Full metadata record
DC FieldValueLanguage
dc.contributor.authorAntia, H. M-
dc.date.accessioned2008-02-23T10:30:50Z-
dc.date.available2008-02-23T10:30:50Z-
dc.date.issued2000-
dc.identifier.citationBASI, Vol. 28, No. 1, pp. 75 - 79en
dc.identifier.urihttp://hdl.handle.net/2248/2038-
dc.description.abstractThe rotation rate in the solar interior can be inferred from measured splittings of solar oscillation frequencies using various inversion techniques. While other large scale flows can be studied using local techniques, like ring diagrams or time-distance helioseismology. These techniques can be used to study variation in flow velocities in the three spatial dimensions as well as the temporal variations.en
dc.format.extent420619 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000BASI...28...75Aen
dc.subjectSun: Oscillationsen
dc.subjectSun: Interioren
dc.subjectSun: Rotationen
dc.titleRotation rate and flows in the solar interioren
dc.typeArticleen
Appears in Collections:BASI Publications

Files in This Item:
File Description SizeFormat 
Antia.pdf410.76 kBAdobe PDFThumbnail
View/Open
Show simple item record


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