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Stellar-solar Activity: How Does It Evolve?тезисы доклада Тезисы
- Автор: Katsova M.
- Сборник: Tenth Workshop "Solar influences on the magnetosphere, ionosphere and atmosphere" Primorsko, Bulgaria, June 4-8, 2018, Book of Abstract
- Тезисы
- Год издания: 2018
- Место издания: Space Research and Technology Institute Bulgaria
- Первая страница: 42
- Последняя страница: 42
- DOI: 10.31401/WSoz.2018.abs
- Аннотация: This invited lecture is presented for participations of the Summer school "Sun, space weather and space climate" held in the framework of the conference: Several observational projects fulfilled during past 25 years allow us to trace changes of activity of sun-like stars throughout all stages of their lives from an epoch of star formation to the age when the cycle becomes regular, and up to the present. We will consider distinctions between saturated activity intrinsic to the youngest fast rotating low-mass stars and solar-type activity typical for older Suns. We discuss frequency of superflares on the Sun and other stars, and a role of local and large-scale magnetic fields in formation of flares. All these points are important for understanding space factors affecting on physical conditions on the Earth and its geo- and biosphere.
- Добавил в систему: Кацова Мария Михайловна