Kane, R. P. (2007) A Preliminary Estimate of the Size of the Coming Solar Cycle 24, based on Ohl’s Precursor Method. Solar Physics, 243 (2). 205-217 doi:10.1007/s11207-007-0475-4

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Reference Type	Journal (article/letter/editorial)
Title	A Preliminary Estimate of the Size of the Coming Solar Cycle 24, based on Ohl’s Precursor Method
Journal	Solar Physics
Authors	Kane, R. P.		Author
Year	2007 (September 25)	Volume	243
Issue	2
Publisher	Springer Science and Business Media LLC
DOI	doi:10.1007/s11207-007-0475-4Search in ResearchGate
	Generate Citation Formats
Mindat Ref. ID	8922795	Long-form Identifier	mindat:1:5:8922795:2
GUID	0
Full Reference	Kane, R. P. (2007) A Preliminary Estimate of the Size of the Coming Solar Cycle 24, based on Ohl’s Precursor Method. Solar Physics, 243 (2). 205-217 doi:10.1007/s11207-007-0475-4
Plain Text	Kane, R. P. (2007) A Preliminary Estimate of the Size of the Coming Solar Cycle 24, based on Ohl’s Precursor Method. Solar Physics, 243 (2). 205-217 doi:10.1007/s11207-007-0475-4
In	(2007, September) Solar Physics Vol. 243 (2) Springer Science and Business Media LLC

	*Kane, R. P. (1997) A preliminary estimate of the size of the coming solar cycle 23, based on Ohl's Precursor Method. Geophysical Research Letters, 24 (15) 1899-1902 doi:10.1029/97gl01932*
	Kane, R. P. (1998) Correction to “A preliminary estimate of the size of the coming solar cycle 23, based on Ohl's Precursor Method”. Geophysical Research Letters, 25 (16) 3121 doi:10.1029/98gl02257
	*Kane, R. P. (2010) Size of the coming solar cycle 24 based on Ohl's Precursor Method, final estimate. Annales Geophysicae, 28 (7) 1463-1466 doi:10.5194/angeo-28-1463-2010*
	*Kane, R. P. (2007) Solar Cycle Predictions based on Solar Activity at Different Solar Latitudes. Solar Physics, 246 (2). 471-485 doi:10.1007/s11207-007-9050-2*
	*Kane, R. P. (2007) Solar Cycle Predictions Based on Extrapolation of Spectral Components: An Update. Solar Physics, 246 (2). 487-493 doi:10.1007/s11207-007-9059-6*
	*Kane, R. P. (2013) An Estimate for the Size of Sunspot Cycle 24. Solar Physics, 282 (1). 87-90 doi:10.1007/s11207-012-0131-5*
	*Kane, R. P. (1989) Maximum sunspot number R z (max) in the coming solar cycle No. 22 ? A revised estimate. Solar Physics, 122 (1). 175-185 doi:10.1007/bf00162833*
	*Kane, R. P. (2007) Latitude Dependence of the “Gnevyshev” Peaks and Gaps. Solar Physics, 245 (2). 415-421 doi:10.1007/s11207-007-9031-5*
	*Lantos, P. (2006) The Skewness of a Solar Cycle as a Precursor of the Amplitude of the Next. Solar Physics, 236 (1). 199-205 doi:10.1007/s11207-006-0145-y*
	*Kane, R. P. (2008) Prediction of Solar Cycle Maximum Using Solar Cycle Lengths. Solar Physics, 248 (1). 203-209 doi:10.1007/s11207-008-9125-8*
	*Maclean, R. C., Priest, E. R. (2007) Topological Aspects of Global Magnetic Field Reversal in the Solar Corona. Solar Physics, 243 (2). 171-191 doi:10.1007/s11207-007-0450-0*

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Kane, R. P. (2007) A Preliminary Estimate of the Size of the Coming Solar Cycle 24, based on Ohl’s Precursor Method. Solar Physics, 243 (2). 205-217 doi:10.1007/s11207-007-0475-4

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