On the p-mode asymmetry between velocity and intensity from the GONG+ data

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dc.creatorTripathy, S. C.
dc.creatorJain, Kiran
dc.creatorHill, Frank
dc.creatorToner, C. G.
dc.date2003-06-02
dc.date.accessioned2026-07-07T02:08:40Z
dc.date.available2026-07-07T02:08:40Z
dc.descriptionWe 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. It is found 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.
dc.description3 pages, Latex (requires Basi.sty), poster paper presented in the annual meeting of ASI (2003)
dc.identifierhttps://arxiv.org/abs/astro-ph/0306027
dc.identifierhttp://arxiv.org/abs/astro-ph/0306027
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6143
dc.subjectAstrophysics
dc.titleOn the p-mode asymmetry between velocity and intensity from the GONG+ data
dc.typetext

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