Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2714
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dc.contributor.authorJavaraiah, J-
dc.date.accessioned2008-07-16T07:36:04Z-
dc.date.available2008-07-16T07:36:04Z-
dc.date.issued2002-09-
dc.identifier.citationBASI, Vol. 30, No. 3, pp. 587 - 588en
dc.identifier.urihttp://hdl.handle.net/2248/2714-
dc.description.abstractPower spectra of N-S asymmetries of the coefficients A and (j of the Sun's surface differential rotation determined from the Mt. Wilson velocity data during 1982-1994 suggest the existence of a period at 374 ± 30 day in the N-8 asymmetries of A and (j with> 99.9% confidence level. The spectrum of the N-S asymmetry of the coefficient lJ suggests existence of the periods at 374 ± 30 day, 78 ± 2 day and 49 ± 1 day in the N-S asymmetry of iJ with ~ 99% confidence level.en
dc.format.extent73489 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectSun: Rotationen
dc.subjectDifferential Rotationen
dc.subjectNorth-South Asymmetryen
dc.titleShort-term periodicities in the north-south asymmetry of the Sun's surface rotationen
dc.typeArticleen
Appears in Collections:BASI Publications

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