Solar models with helioseismologically correct sound speed profile

dc.contributor.author	Ajukov, S. V
dc.contributor.author	Baturin, V. A
dc.date.accessioned	2007-09-21T10:25:17Z
dc.date.available	2007-09-21T10:25:17Z
dc.date.issued	1996
dc.identifier.citation	BASI, Vol.24 No. 2 pp. 329-332	en
dc.identifier.uri	http://hdl.handle.net/2248/1817
dc.description.abstract	The problem of computation of the model of the present Sun with given sound speed profile in the solar radiative zone is considered. It is shown that the chemical composition is still a free parameter but the entropy of the adiabatic part of the convection zone is determined by this procedure. Parameters of the models are compared with the helioseismic calibration of solar envelope and the disagreement is revealed. A study of the seismic properties of the models' cores indicates that the best model is the one closest to the standard solar model.	en
dc.format.extent	299493 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..329A	en
dc.subject	Solar interior	en
dc.subject	Helioseismology	en
dc.title	Solar models with helioseismologically correct sound speed profile	en
dc.type	Article	en