Solar structure as revealed by 1 year LOWL data

dc.contributor.author	Basu, S
dc.contributor.author	Christensen-Dalsgaard, J
dc.contributor.author	Schou, J
dc.contributor.author	Thompson, M. J
dc.contributor.author	Tomczyk, S
dc.date.accessioned	2007-09-19T06:46:01Z
dc.date.available	2007-09-19T06:46:01Z
dc.date.issued	1996
dc.identifier.citation	BASI, Vol.24 No. 2 pp. 147-150	en
dc.identifier.uri	http://hdl.handle.net/2248/1802
dc.description.abstract	We have used solar frequencies obtained form 1 year of observations with LOWL instrument to investigate the radial stratification of the Sun. Models which include the diffusion of helium and heavy elements below the solar convection zone are found to have a structure much closer to that of the Sun than models without diffusion. Also, models constructed with the Livermore(OPAL)equation of state seem to match the real Sun better than models constructed with the MHD equation of state. Finally, we find that an increase in the value of Z/X reduces the difference between models and Sun.	en
dc.format.extent	328939 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..147B	en
dc.subject	Sun	en
dc.subject	Interior - Sun	en
dc.subject	Oscillations - Diffusion	en
dc.title	Solar structure as revealed by 1 year LOWL data	en
dc.type	Article	en