Using solar oscillations to constrain the equation of state and low-temperature opacities

dc.contributor.author	Guzik, J. A
dc.contributor.author	Cox, A. N
dc.contributor.author	Swenson, F. J
dc.date.accessioned	2007-09-19T07:24:57Z
dc.date.available	2007-09-19T07:24:57Z
dc.date.issued	1996
dc.identifier.citation	BASI, Vol.24 No. 2 pp. 161-170	en
dc.identifier.uri	http://hdl.handle.net/2248/1804
dc.description.abstract	Because 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 oscillations	en
dc.format.extent	817365 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1996BASI...24..161G	en
dc.subject	Sun: oscillations	en
dc.subject	Sun: interior	en
dc.subject	Sun: diffusion	en
dc.subject	Sun: evolution	en
dc.title	Using solar oscillations to constrain the equation of state and low-temperature opacities	en
dc.type	Article	en