Solar cycle variation in GONG and MDI data: 1995-2002

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dc.creatorTripathy, S. C.
dc.date2003-06-02
dc.date.accessioned2026-07-07T02:08:40Z
dc.date.available2026-07-07T02:08:40Z
dc.descriptionBoth GONG and MDI projects have measured {\it 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 frequencies and splitting coefficients.
dc.description6 pages, Latex (requires Basi.sty), invited review presented in the annual meeting of ASI (2003)
dc.identifierhttps://arxiv.org/abs/astro-ph/0306028
dc.identifierhttp://arxiv.org/abs/astro-ph/0306028
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6144
dc.subjectAstrophysics
dc.titleSolar cycle variation in GONG and MDI data: 1995-2002
dc.typetext

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