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The activity of the solar atmosphere and solar-type stars at 11-year and quasi-biennial timescalesстатья
Информация о цитировании статьи получена из
Web of Science,
Scopus
Статья опубликована в журнале из списка Web of Science и/или Scopus
Дата последнего поиска статьи во внешних источниках: 6 сентября 2017 г.
- Авторы: Bruevich E.A., Kononovich E.V.
- Журнал: Moscow University Physics Bulletin
- Том: 66
- Номер: 1
- Год издания: 2011
- Издательство: Allerton Press
- Местоположение издательства: New York, N.Y., United States
- Первая страница: 72
- Последняя страница: 77
- DOI: 10.3103/S0027134911010073
- Аннотация: We studied new simultaneous observations of the flux variations of the photospheric and chromospheric emissions of 33 solar-type stars and Sun during the HK-project that were conducted over the past 20 years. In addition to the known cyclic chromospheric emission variations of stars at the 11-year time scale, which were discovered at the Mount Wilson Observatory, we found a recurrences that are similar to the quasi-biennial variations of solar radiation. The results of calculations of the radiation fluxes variations periods of stars at the quasi-biennial scale are given.
- Добавил в систему: Бруевич Елена Александровна