Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5031
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dc.contributor.authorGokhale, M. H-
dc.date.accessioned2010-02-24T11:04:04Z-
dc.date.available2010-02-24T11:04:04Z-
dc.date.issued1979-11-
dc.identifier.citationKodaikanal Observatory Bulletins Series A, Vol. 2, No. 3, pp 222–223en
dc.identifier.issn0374-3632-
dc.identifier.urihttp://hdl.handle.net/2248/5031-
dc.description.abstractThe two component nature of the solar activity cycle as resulting from the shock-transition model of the solar magnetic cycle, provides for a correlation between a measure of coronal hole formations during the ending years of one solar cycle and the maximum annual sunspot number R/submax of the next cycle. This might account for the observed correlation between the geomagnetic activity during the last few years of one cycle and the R/submax of the next cycle.en
dc.language.isoenen
dc.publisherIndian Institute of Astrophysicsen
dc.rights© Indian Institute of Astrophysicsen
dc.subjectSolar Cycleen
dc.subjectSolar Magnetic Fieldsen
dc.subjectGeomagnetic Activityen
dc.subjectSolar Cycle Theoryen
dc.titleWhy is geomagnetic activity during the ending years of a solar cycle well correlated to the maximum of the next cycle?en
dc.typeArticleen
Appears in Collections:Kodaikanal Observatory Bulletins (1905 - 1997 )
IIAP Publications

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