SOLAR CYCLE STRUCTURE AND STRUCTURE OF ACTIVITY CYCLES AT LATE TYPE STARES

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Resumo

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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Sobre autores

V. Obridko

IZMIRAN

Autor responsável pela correspondência
Email: obridko@izmiran.ru
Russia, Troitsk

D. Sokoloff

IZMIRAN; Lomonosov Moscow State University

Email: obridko@izmiran.ru
Russia, Troitsk; Russia, Moscow

M. Katsova

Lomonosov Moscow State University, Sternberg Astronomical Institute

Email: obridko@izmiran.ru
Russia, Moscow

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Declaração de direitos autorais © В.Н. Обридко, Д.Д. Соколов, М.М. Кацова, 2023