GONG p-mode frequency changes with solar activity

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DC Field	Value	Language
dc.contributor.author	Bhatnagar, A	-
dc.contributor.author	Jain, K	-
dc.contributor.author	Tripathy, S. C	-
dc.date.accessioned	2008-02-23T10:58:35Z	-
dc.date.available	2008-02-23T10:58:35Z	-
dc.date.issued	2000	-
dc.identifier.citation	BASI, Vol. 28, No. 1, pp. 91 - 92	en
dc.identifier.uri	http://hdl.handle.net/2248/2042	-
dc.description.abstract	In this paper, we present a correlation study of nine solar activity indices with p-mode frequency shifts obtained from the GONG data. It is found that the two are closely correlated and a linear relationship exits. Further, the GONG p-mode frequencies for the period 1995 August to 1997 August show that the mean frequency decreases by 0.06 μHz during the descending phase of the solar cycle 22 and increases by 0.04 μHz in the ascending phase of the new solar cycle 23.	en
dc.format.extent	143172 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...91B	en
dc.subject	Sun: Oscillations	en
dc.subject	Sun: activity	en
dc.title	GONG p-mode frequency changes with solar activity	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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