Solar Cycle Variation in GONG and MDI Data : 1995-2002

dc.contributor.author	Tripathy, S. C
dc.date.accessioned	2008-05-27T09:19:41Z
dc.date.available	2008-05-27T09:19:41Z
dc.date.issued	2003
dc.identifier.citation	BASI, Vol. 31, No. 3&4, pp. 153 - 158	en
dc.identifier.uri	http://hdl.handle.net/2248/2352
dc.description.abstract	Both GONG and MDI projects have measured p-mode frequencies of the Sun for more than 7 years. Here we review what we have learnt from the temporal variation of the oscillation frequencie and splitting coefficients.	en
dc.format.extent	233264 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/2003BASI...31..153T	en
dc.subject	Sun	en
dc.subject	Helioseismology	en
dc.subject	MDI Data	en
dc.title	Solar Cycle Variation in GONG and MDI Data : 1995-2002	en
dc.type	Article	en