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Long term periodicities in the sunspot cycle

Abstract

THE existence of a long period undulation (179 yr) in the solar cycle (Fig. 1, based on data from Waldmeier1,2 is suggested by the planetary theory of sunspots. Jose3, for example, postulated an association between the 178.8-yr periodicity in orbital positions of the planets and the phase of the solar cycle. Wood4 used the presumed existence of a cycle of 170–180 yr in solar activity to predict the peak dates of future sunspot cycles. Our work indicates that although a 179-yr periodicity does exist in the sunspot cycle, it is not caused by a primary long term excitation function but is, instead, a beat phenomenon. This can be seen by computing the spectrum for the data shown in Fig. 1.

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References

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COHEN, T., LINTZ, P. Long term periodicities in the sunspot cycle. Nature 250, 398–400 (1974). https://doi.org/10.1038/250398a0

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  • DOI: https://doi.org/10.1038/250398a0

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