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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2352
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dc.contributor.authorTripathy, S. C-
dc.date.accessioned2008-05-27T09:19:41Z-
dc.date.available2008-05-27T09:19:41Z-
dc.date.issued2003-
dc.identifier.citationBASI, Vol. 31, No. 3&4, pp. 153 - 158en
dc.identifier.urihttp://hdl.handle.net/2248/2352-
dc.description.abstractBoth GONG and MDI projects have measured p-mode frequencies of the Sun for more than 7 years. Here we review what we have learnt from the temporal variation of the oscillation frequencie and splitting coefficients.en
dc.format.extent233264 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2003BASI...31..153Ten
dc.subjectSunen
dc.subjectHelioseismologyen
dc.subjectMDI Dataen
dc.titleSolar Cycle Variation in GONG and MDI Data : 1995-2002en
dc.typeArticleen
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