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Eight types of the solar wind and their originsстатья
- Авторы: Veselovsky I.S., Kaportseva K.B., Lukashenko A.T.
- Сборник: Workshop “Solar Influences on the Magnetosphere, Ionosphere and Atmosphere”. Book of Proceedings. Ninth Workshop. Sunny Beach, Bulgaria, May 30 – June 3, 2017
- Серия: ISSN 2367–7570
- Год издания: 2017
- Место издания: Bulgaria
- Первая страница: 24
- Последняя страница: 28
- Аннотация: In July 2016 high cadence data from the new DSCOVR satellite, launched at the Lagrange point in February 2015, became available. On the basis of these data a binary (large-small) three-parameter classification of solar wind types, according to the main hydrodynamic parameters (speed, density and temperature), is presented, and examples of the determination of different types of solar wind in real time are given. We get eight types of solar wind: fast-hot-dense, fast-hot-rarefied, fast-cold-dense, fast-cold-rarefied, slow-hot-dense, slow-hot-rarefied, slow-cold-dense, slow-cold-rarefied, comparing to some average values for given time intervals. These types occur at different frequencies and represent consequences of different solar activity sorts. The most interesting situations correspond to extreme values because of magnetospheric effects. This report considers possible solar “sources” of listed types.
- Добавил в систему: Лукашенко Анастасия Тарасовна