Why is geomagnetic activity during the ending years of a solar cycle well correlated to the maximum of the next cycle?

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5031

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DC Field	Value	Language
dc.contributor.author	Gokhale, M. H	-
dc.date.accessioned	2010-02-24T11:04:04Z	-
dc.date.available	2010-02-24T11:04:04Z	-
dc.date.issued	1979-11	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 2, No. 3, pp 222–223	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/5031	-
dc.description.abstract	The 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.iso	en	en
dc.publisher	Indian Institute of Astrophysics	en
dc.rights	© Indian Institute of Astrophysics	en
dc.subject	Solar Cycle	en
dc.subject	Solar Magnetic Fields	en
dc.subject	Geomagnetic Activity	en
dc.subject	Solar Cycle Theory	en
dc.title	Why is geomagnetic activity during the ending years of a solar cycle well correlated to the maximum of the next cycle?	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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