Abstract
It is shown that the use of a description of the solar cycle that takes into account the odd zonal harmonic of the solar magnetic field allows us to deepen our knowledge of two important aspects of solar activity: first, to clarify and expand predictions for the near future of the evolution of the cyclic activity of the Sun, second, to formulate a program for monitoring the spectrophotometric characteristics of the radiation of stars like the Sun, aimed at obtaining new information about their magnetic fields.
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