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

V. N. Obridko; Обридко В. Н.; D. D. Sokoloff; Соколов Д. Д.; M. M. Katsova; Кацова М. М.

doi:10.31857/S000462992312006X

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

作者: Obridko V.N.¹, Sokoloff D.D.¹^,2, Katsova M.M.³
隶属关系:
1. IZMIRAN
2. Lomonosov Moscow State University
3. Lomonosov Moscow State University, Sternberg Astronomical Institute
期: 卷 100, 编号 12 (2023)
页面: 1311-1321
栏目: Articles
URL: https://journals.rcsi.science/0004-6299/article/view/233474
DOI: https://doi.org/10.31857/S000462992312006X
EDN: https://elibrary.ru/CZRBNF
ID: 233474

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详细

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.

关键词

solar cycle, late type stars

参考

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