The most recent solar cycle, currently estimated to have reached a minimum in December 2008 based on a 12 month centered moving average of monthly sunspot numbers, was the longest solar cycle since 1798‐1810, measured trough to trough. The cycle lasted approximately 150 months or 12.5 years, two full years longer than the 20th century average of 10.5 years. The impact of a long solar cycle is twofold. First of all, there is a definite correlation between the length of one solar cycle and the peak sunspot number during the following cycle as the graph below shows.
Only two solar cycles since 1750 have lasted as long as or longer than the most recent cycle, and both were followed by the weakest solar maximums of the past 250 years, a period during the early 1800s known as the Dalton Minimum. Given the length of the previous cycle, the upcoming solar cycle could be among the weakest on record since 1750 if the relationship holds. Additionally, of the last five solar cycles that persisted twelve or more months longer than average, four were followed by another cycle lasting longer than average. In every instance, however, the next solar cycle was somewhat shorter in length than the previous cycle.
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