SOLAR CYCLE STRUCTURE AND STRUCTURE OF ACTIVITY CYCLES AT LATE-TYPE STARSстатья
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Дата последнего поиска статьи во внешних источниках: 10 апреля 2024 г.
Аннотация:It is shown that a description of the solar cycle using the odd zonal harmonic of the solar magnetic field expands our capabilities in two important areas of solar research: first, in improving and expanding the forecast to the near future of evolution of the cyclic solar activity and, second, in developing a program for monitoring the spectrophotometric characteristics of radiation of solar-like stars, aimed at obtaining new information about their magnetic fields.