Abstract

A periodogram device was applied to the sunspot series  $X^*_t$ . The analysis resulted in a period estimate of  $10.8\approx 11$ years. The periodogram was displayed graphically and the largest peak corresponded to a frequency of $0.0926$. A significant test on randomness of the series was also carried out to ascertain this result. It was observed that the period 10.8 which accounted for 80.68\% of the variance of  $X_t$ was statistically significant at the 0.05 level.

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