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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1821
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dc.contributor.authorJavaraiah, J-
dc.date.accessioned2007-09-25T07:14:24Z-
dc.date.available2007-09-25T07:14:24Z-
dc.date.issued1996-
dc.identifier.citationBASI, Vol.24 No. 2 pp. 351-354en
dc.identifier.urihttp://hdl.handle.net/2248/1821-
dc.description.abstractRecently, we studied the rotaion of sunspot gruoups during 1879-1976 and detected ~ 22-yr and a few more other periods 'even' and 'odd' parity torsional oscillations of the Sun (Javaraiah & Gokhale 1995a, b). In the present paper we show that the amplitudes of these torsional oscillations of the Sun depend upon the temporal variation in the latitude (celestial) distribution of angular momentum of the solar system.en
dc.format.extent371971 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1996BASI...24..351Jen
dc.subjectSolar rotationen
dc.subjectMagnetic fielden
dc.subjectActivity cycleen
dc.subjectSolar system dynamicsen
dc.titlePeriodicities in the Sun's "Torsional MHD oscillations" and planetary configurationsen
dc.typeArticleen
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