Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3314
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dc.contributor.authorJavaraiah, J-
dc.contributor.authorGokhale, M. H-
dc.date.accessioned2008-09-02T10:31:05Z-
dc.date.available2008-09-02T10:31:05Z-
dc.date.issued1997-02-
dc.identifier.citationSolar Physics, Vol. 170, No. 2, pp. 389 - 410en
dc.identifier.issn0038-0938-
dc.identifier.urihttp://hdl.handle.net/2248/3314-
dc.descriptionRestricted Accessen
dc.description.abstractWe have studied the temporal variations in the north–south asymmetries of the differential rotation parameters A, B, and the mean rotation rate , by determining their values from Greenwich data for sunspot groups (1879–1976) in the northern and southern hemispheres, during moving time intervals of lengths 3 yr and 5 yr, successively displaced by 1 yr. The variation in the north–south asymmetry (A a) of is similar to the variation in the asymmetry (B ) of B but with opposite sign. These variations of and B may represent components of an anti-symmetric torsional oscillation which are in opposite phase with each other. The FFT and MEM analyses of the temporal variations of B , , and the north–south asymmetry (A ) of A, show existence of significant periodicities: 45.5 ± 11.5 yr,21.3 ± 4.5 yr, 13.3 ± 1.5 yr, and 10.5 ± 0.5 yr. These analyses also show a few other possible periodicities in A , B , and . All these periodicities are also seen in the north–south asymmetry of sunspot activity (with similar relative magnitudes). The 22-yr periodicity was seen in even-parity modes of magnetic field inferred from sunspot data.en
dc.language.isoenen
dc.publisherSpringeren
dc.relation.urihttp://www.springerlink.com/content/wlu38m07hjp153k8/en
dc.subjectDifferential Rotation Parametersen
dc.subjectSunspot Groupsen
dc.subjectSunspot Activityen
dc.subjectRelative Magnitudesen
dc.subjectMagnetic Field Inferreden
dc.titlePeriodicities in the North–South Asymmetry of the Solar Differential Rotation and Surface Magnetic Fielden
dc.typeArticleen
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