STELLAR ACTIVITY CYCLES: WHY DO WE NEED IN THE LONG-TERM MEASUREMENTS OF THE MAGNETIC FIELD?

Автор(и)

  • S. I. Plachinda Crimean Astrophysical Observatory, Nauchny, Crimea, Україна
  • V. V. Butkovskaya Main Astronomical Observatory of National Academy of Sciences, Україна

DOI:

https://doi.org/10.18524/1810-4215.2017.30.114374

Ключові слова:

stars, activity, late-type stars, magnetic fields

Анотація

Solution of the two important problems requires a study of long-term behavior of the magnetic field on stars with nondegenerate matter: firstly, to define the role of the magnetic field on different evolutionary stages of stars; secondly, to know the influence of the star’s activity on space weather in the habitable zone. This brief review summarizes the first results of the long-term magnetic field measurements on selected stars.

Посилання

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Опубліковано

2017-11-08

Номер

Розділ

Астрофізика (зоряні атмосфери, взаємодіючі подвійні системи, змінні зорі)