Interpretation of the 'third harmonic' of the solar magnetic cycle

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3530

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DC Field	Value	Language
dc.contributor.author	Gokhale, M. H	-
dc.contributor.author	Javaraiah, J	-
dc.date.accessioned	2008-09-10T12:30:52Z	-
dc.date.available	2008-09-10T12:30:52Z	-
dc.date.issued	1990	-
dc.identifier.citation	IAU Symposium, No. 142, pp. 119 - 123	en
dc.identifier.issn	0074-1809	-
dc.identifier.uri	http://hdl.handle.net/2248/3530	-
dc.description.abstract	The behavior and significance of a third harmonic peak at about 3/22/y which is present in the spectra of all the odd degree axisymmetric modes with respect to the temporal frequency are investigated. The correlation between the amplitudes and phases of the third harmonic components and those of the corresponding first harmonic components is determined. The presence of high correlation between the amplitudes of the first and third harmonics shows that the third harmonic peaks do not represent any independent periodicity.	en
dc.language.iso	en	en
dc.publisher	International Astronomical Union	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1990IAUS..142..119G	en
dc.subject	Fourier analysis	en
dc.subject	Solar cycles	en
dc.subject	Solar magnetic field	en
dc.subject	Spherical harmonics	en
dc.subject	Sunspots	en
dc.subject	Solar rotation	en
dc.subject	Spectroheliographs	en
dc.title	Interpretation of the 'third harmonic' of the solar magnetic cycle	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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