Seismic investigation of the solar structure using GONG frequencies

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dc.creatorTripathy, S. C.
dc.creatorAntia, H. M.
dc.creatorHill, F.
dc.creatorAmbastha, A.
dc.date1997-03-27
dc.date.accessioned2026-07-07T02:23:06Z
dc.date.available2026-07-07T02:23:06Z
dc.descriptionUsing the recently obtained GONG frequencies, we investigate the properties of the solar interior by constructing solar models with various input physics like opacities, equation of state, nuclear reaction rates etc. The differential asymptotic inversion technique is then used to infer the relative difference in sound speed between the Sun and solar models. Here we apply these results to test equation of state and different formulation for calculating the convective flux.
dc.descriptionLatex, 2 pages, 3 figures, To appear in the IAU Symp. # 181: "Sounding solar and stellar interiors", eds. F.X. Schmider & J. Provost
dc.identifierhttps://arxiv.org/abs/astro-ph/9703179
dc.identifierhttp://arxiv.org/abs/astro-ph/9703179
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11123
dc.subjectAstrophysics
dc.titleSeismic investigation of the solar structure using GONG frequencies
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