Effects on solar structure of opacity changes

dc.contributor.author	Tripathy, S. C
dc.contributor.author	Christensen-Dalsgaard, J
dc.date.accessioned	2007-09-17T10:56:17Z
dc.date.available	2007-09-17T10:56:17Z
dc.date.issued	1996
dc.identifier.citation	BASI, Vol. 24, No. 2, pp. 129-132	en
dc.identifier.uri	http://hdl.handle.net/2248/1798
dc.description.abstract	We investigate the sensitivity of solar structure to localized changes in opacity by considering differences between models computed with locally modified opacity and unmodified references models. The results confirm that the sound-speed differences are small in most of the convection zone. Assuming that the linear approximation is valid, we further show that these differences can be reproduced by constructing envelope models with the same input physical parameters as the original model.	en
dc.format.extent	275523 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..129T	en
dc.subject	solar structure	en
dc.subject	solar oscillations	en
dc.subject	opacity	en
dc.title	Effects on solar structure of opacity changes	en
dc.type	Article	en