The seismic sun

dc.contributor.author	Basu, S
dc.date.accessioned	2008-02-23T07:41:01Z
dc.date.available	2008-02-23T07:41:01Z
dc.date.issued	2000
dc.identifier.citation	BASI, Vol. 28, No. 1, pp. 63 - 69	en
dc.identifier.uri	http://hdl.handle.net/2248/2036
dc.description.abstract	The "Seismic Sun" is a model of the Sun constructed using helioseismological deductions about the Sun. The seismic Sun is very similar to a standard solar model which incorporates gravitational settling of helium and heavy elements. The main discrepancy is just below the base of the convection zone and can be attributed to the lack of mixing in standard solar models.	en
dc.format.extent	593434 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/2000BASI...28...63B	en
dc.subject	Sun: Oscillations	en
dc.subject	Sun: Interior	en
dc.title	The seismic sun	en
dc.type	Article	en