Rotation rate and flows in the solar interior

dc.contributor.author	Antia, H. M
dc.date.accessioned	2008-02-23T10:30:50Z
dc.date.available	2008-02-23T10:30:50Z
dc.date.issued	2000
dc.identifier.citation	BASI, Vol. 28, No. 1, pp. 75 - 79	en
dc.identifier.uri	http://hdl.handle.net/2248/2038
dc.description.abstract	The rotation rate in the solar interior can be inferred from measured splittings of solar oscillation frequencies using various inversion techniques. While other large scale flows can be studied using local techniques, like ring diagrams or time-distance helioseismology. These techniques can be used to study variation in flow velocities in the three spatial dimensions as well as the temporal variations.	en
dc.format.extent	420619 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...75A	en
dc.subject	Sun: Oscillations	en
dc.subject	Sun: Interior	en
dc.subject	Sun: Rotation	en
dc.title	Rotation rate and flows in the solar interior	en
dc.type	Article	en