Periodicities in the Sun's "Torsional MHD oscillations" and planetary configurations

dc.contributor.author	Javaraiah, J
dc.date.accessioned	2007-09-25T07:14:24Z
dc.date.available	2007-09-25T07:14:24Z
dc.date.issued	1996
dc.identifier.citation	BASI, Vol.24 No. 2 pp. 351-354	en
dc.identifier.uri	http://hdl.handle.net/2248/1821
dc.description.abstract	Recently, 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.extent	371971 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/1996BASI...24..351J	en
dc.subject	Solar rotation	en
dc.subject	Magnetic field	en
dc.subject	Activity cycle	en
dc.subject	Solar system dynamics	en
dc.title	Periodicities in the Sun's "Torsional MHD oscillations" and planetary configurations	en
dc.type	Article	en