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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2406
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dc.contributor.authorTripathy, S. C-
dc.contributor.authorJain, K-
dc.contributor.authorHill, F-
dc.contributor.authorToner, C. G-
dc.date.accessioned2008-06-05T09:59:30Z-
dc.date.available2008-06-05T09:59:30Z-
dc.date.issued2003-
dc.identifier.citationBASI, Vol. 31, No. 3&4, pp. 321 - 323en
dc.identifier.urihttp://hdl.handle.net/2248/2406-
dc.description.abstractWe have analyzed the local acoustic spectra of small regions over the solar surface at different locations from disk center to limb via the technique of ring diagrams. The analysis suggest that the frequency shifts between velocity and intensity is a function of location on the disk and is higher near the disk center than those near the limb.en
dc.format.extent90266 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2003BASI...31..321Ten
dc.subjectSolar oscillationen
dc.subjectIntensityen
dc.subjectGONG+en
dc.titleOn the p-mode Asymmetry between Velocity and Intensity from the GONG+ Dataen
dc.typeArticleen
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