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MAGNETIC FIELD STRUCTURE AND SOLAR WIND STREAMS NEAR SOLAR MAXIMUM OF 2012 доклад на конференции
- Авторы: Shugay Yu S., Veselovsky I.S., Slemzin V.A.
- Международная Конференция : The sun: quiet and active — 2013, International Moscow Workshop on Solar Physics
- Даты проведения конференции: 2013
- Тип доклада: Устный
- Докладчик: Shugay Yu S.
- Место проведения: Moscow, Russia, Russia
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Аннотация доклада:
The structure and evolution of global coronal magnetic field, a long-living CH, the sector structure of IMF and parameters of SW streams near solar cycle 24 maximum were considered. We compare global coronal field patterns with the sources of the SW and “in situ” observations near the Earth’s orbit. Fast SW density flux is associated with a large CH and high-speed sporadic events Slow solar wind density flux shows the best correlation with the total areas of several small CHs.
- Добавил в систему: Шугай Юлия Сергеевна