Prediction of Sunspot Numbers until the End of the Present Cycle

Physics

Scientific paper

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Scientific paper

SINCE November 1956 the use of a most elementary long-term prediction
method1 for sunspot numbers has been pursued with surprising
success. C. N. Anderson2 directed attention to the possible
existence of a 169 years period in solar activity. The coincidence of
values between the two periods 1749-85 and 1918-54 is most striking.

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