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On the global magnetic activity and dynamo of the Sun and solar-type starsстатья
- Авторы: Bruevich E.A., Rozgacheva I.K.
- Сборник: Solar and Stellar Astrophysics ArXiv (astro-ph.SR)
- Серия: № 5705B
- Том: 8
- Год издания: 2012
- Место издания: (astro-ph.SR)
- Первая страница: 1
- Последняя страница: 12
- Аннотация: The activity of the Sun as a result of cyclic changes of the global magnetic field is studied. As a consequence of the analysis of magnetic activity of solar-type stars the following power dependencies were found: the dependence between the rotation periods and the effective temperatures, the dependence between the duration of the "11-year" cycles of activity and the effective temperatures, and the dependence between the duration of quasi-biennial cycles and the effective temperatures. It is shown that the physical nature of these dependencies associated with the observed properties of solar-type stars and can be explained by the existence of internal Rossby waves around the base of convective shells of these stars.
- Добавил в систему: Бруевич Елена Александровна