A NOTE ON SOLAR ACTIVITY AND PREDICTIONS
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Graphical Abstract
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Abstract
It is generally accepted that for the maximum of solar cycle 21 only a few statistical methods gave predictions near the observed value. Comparing predictions for cycle 22 1 with the observed data of sunspot numbers given in SESC PRF of SGD2 a general same tendency as for the cycle 21 can easily be found. A research of properties of solar cycles would be helpful for the improving of our predictions.
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