NASA NTRS · 19780053157
Using dynamo theory to predict the sunspot number during solar cycle 21
Abstract
On physical grounds it is suggested that the polar field strength of the sun near a solar minimum is closely related to the solar activity of the following cycle. Four methods of estimating the polar magnetic field strength of the sun near solar minimum are employed to provide an estimate of the yearly mean sunspot number of cycle 21 at solar maximum of 140 + or - 20. This estimate may be considered a first-order attempt to predict the cycle activity using one parameter of physical importance based upon dynamo theory.
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Schatten, K. H., Scherrer, P. H., Svalgaard, L., Wilcox, J. M.. 1978-05-01. Using dynamo theory to predict the sunspot number during solar cycle 21. https://ntrs.nasa.gov/citations/19780053157
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