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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1804
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dc.contributor.authorGuzik, J. A-
dc.contributor.authorCox, A. N-
dc.contributor.authorSwenson, F. J-
dc.date.accessioned2007-09-19T07:24:57Z-
dc.date.available2007-09-19T07:24:57Z-
dc.date.issued1996-
dc.identifier.citationBASI, Vol.24 No. 2 pp. 161-170en
dc.identifier.urihttp://hdl.handle.net/2248/1804-
dc.description.abstractBecause thousands of solar p-mode oscillation frequencies have been measured to high accuracy, direct comparisons between calculated and observed frequencies are an excellent means of testing solar interior physics. Here we compare observed and calculated nonadiabatic frequencies of solar models that include diffusive settling of helium and heavier elements. We consider the effects of low-temperature opacities, equation of state, and a nonequilibrium radiation diffusion treatment on solar structure and oscillationsen
dc.format.extent817365 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1996BASI...24..161Gen
dc.subjectSun: oscillationsen
dc.subjectSun: interioren
dc.subjectSun: diffusionen
dc.subjectSun: evolutionen
dc.titleUsing solar oscillations to constrain the equation of state and low-temperature opacitiesen
dc.typeArticleen
Appears in Collections:BASI Publications

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