Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2404
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dc.contributor.authorJavaraiah, J-
dc.date.accessioned2008-06-05T07:32:12Z-
dc.date.available2008-06-05T07:32:12Z-
dc.date.issued2003-
dc.identifier.citationBASI, Vol. 31, No. 3&4, pp. 317 - 318en
dc.identifier.urihttp://hdl.handle.net/2248/2404-
dc.description.abstractUsing the daily Mt. Wilson velocity data during 1986-1994, we found 1.3 ± 0.1 yr periodicity - is dominant in the Sun's surface `mean' rotation rate (A ) during 1986-1994 (solar cycle 22). A 153 ± 5 - day periodicity found to be substantially significant in A during the decay phase of solar cycle 22.en
dc.format.extent62401 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2003BASI...31..317Jen
dc.subjectSun :surface rotationen
dc.subjectSolar activityen
dc.title`1.3-Year' and `153-day' Periodicities in the Sun's Surface Rotationen
dc.typeArticleen
Appears in Collections:BASI Publications

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