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Changes of the Chromospheric network with solar cycle phaseстатья
- Авторы: Kozlova L.M., Somov B.V.
- Журнал: Astronomicheskii Tsirkulyar
- Том: 1589
- Год издания: 2013
- Первая страница: 1
- Последняя страница: 6
- Аннотация: The structure of the coronal holes and their environment as a probable source of high-speed solar wind are investigated. The changes of the sizes and contrasts of the chromospheric network with 11-year cycle phase are discovered from results of the electrophotometric scanning of the solar disc in the IR-lines HeI 10830A as inside coronal holes both on their boundaries and in quiescent solar regions.
- Добавил в систему: Сомов Борис Всеволодович