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22-year periodicity in solar rotation, solar wind parameters and earth rotation

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dc.contributor.author Kirov, B
dc.contributor.author Georgieva, K
dc.contributor.author Javaraiah, J
dc.date.accessioned 2009-06-29T10:17:56Z
dc.date.available 2009-06-29T10:17:56Z
dc.date.issued 2002-12
dc.identifier.citation A. Wilson., ed., Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, ESA SP-506, Vol. 1. Noordwijk: ESA Publications Division, 9 - 14 September 2002, Prague, Czech Republic. pp. 149 - 152 en
dc.identifier.isbn 92-9092-816-6
dc.identifier.uri http://hdl.handle.net/2248/4597
dc.description.abstract It is generally accepted that the annual variation in the Earth's rotation rate is fully determined by large-scale seasonal changes in atmospheric circulation, while the decadal changes in Earth's rotation have been shown to be closely correlated to the North-South asymmetry in solar differential rotation. In the present paper we demonstrate that the oscillations of both the Earth's and the solar rotation rates are different in cycles with negative end positive solar polarity. We find that differences between positive and negative polarity solar cycles exist also in solar wind velocity and interplanetary magnetic field parameters, and suggest that the solar wind mediates the transfer of angular momentum from the Sun to the Earth. en
dc.language.iso en en
dc.publisher European Space Agency en
dc.relation.ispartofseries ESA SP;No. 506
dc.relation.uri http://adsabs.harvard.edu/abs/2002ESASP.506..149K en
dc.subject Solar Activity Cycles: Solar Rotation en
dc.subject Solar Wind en
dc.subject Earth Rotation en
dc.title 22-year periodicity in solar rotation, solar wind parameters and earth rotation en
dc.type Article en


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