Helioseismology

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/182

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DC Field	Value	Language
dc.contributor.author	Antia, H. M	-
dc.date.accessioned	2005-01-08T04:45:18Z	-
dc.date.available	2005-01-08T04:45:18Z	-
dc.date.issued	1988	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 9, pp. 7-20	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/182	-
dc.description.abstract	Many of the oscillations observed at the solar surface have been identified with resonant normal modes of the entire solar body. Accurate measurements of frequencies of these modes enable us to study the internal structure and dynamics of the Sun. Helioseismology has provided a handle to measure the depth of the convection zone and the primordial helium abundance, as well as the sound speed and the rotation velocity throughout much of thesolar interior.	en
dc.format.extent	564799 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Helioseismology	en
dc.subject	Solar Surface	en
dc.title	Helioseismology	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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