Abstract
On the basis of published Wolf Numbers and Schove Row, solar activity cycles in the interval of 11 to hundreds of years have been investigated. In this case the method of investigation of pulsating stars showing the Blazhko effect was applied. The elements of cycles and O-C were calculated and compared with results of solar activity parameters determined by classical methods.
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References
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Romanov, Y.S., Zgonyaiko, N.S. The periodicity of solar activity cycles. Sol Phys 152, 31–34 (1994). https://doi.org/10.1007/BF01473179
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DOI: https://doi.org/10.1007/BF01473179