Dependence of SSNM on SSNm - a Reconsideration for Predicting the Amplitude of a Sunspot Cycle

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3086

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DC Field	Value	Language
dc.contributor.author	Ramesh, K. B	-
dc.date.accessioned	2008-08-12T09:20:03Z	-
dc.date.available	2008-08-12T09:20:03Z	-
dc.date.issued	2000-12	-
dc.identifier.citation	Solar Physics, Vol. 197, No. 2, pp. 421 – 424	en
dc.identifier.issn	0038-0938	-
dc.identifier.uri	http://hdl.handle.net/2248/3086	-
dc.description	Restricted Access	en
dc.description.abstract	An improved correlation between maximum sunspot number (SSNM) and the preceding minimum (SSNm) is reported when the monthly mean sunspot numbers are smoothed with a 13-month running window. This relation allows prediction of the amplitude of a sunspot cycle by making use of the sunspot data alone. The estimated smoothed maximum sunspot number (126+/-26) and time of maximum epoch (second half of 2000) of cycle 23 are in good agreement with the predictions made by some of the precursor methods.	en
dc.format.extent	35188 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.uri	http://www.springerlink.com/content/h401585521x31673/	en
dc.subject	Sunspot Cycle	en
dc.subject	Dependence of SSNM on SSNm	en
dc.title	Dependence of SSNM on SSNm - a Reconsideration for Predicting the Amplitude of a Sunspot Cycle	en
dc.type	Article	en
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