|
ИСТИНА |
Войти в систему Регистрация |
ИПМех РАН |
||
3D evolution of solar magnetic fields and high-speed solar wind streams near the minimum of solar cycle 23статья
Информация о цитировании статьи получена из
Web of Science
Дата последнего поиска статьи во внешних источниках: 27 мая 2015 г.
- Авторы: Yakovchouk O.S., Veselovsky I.S., Mursula K., Shugai Y.S.
- Сборник: IAU Symposium
- Серия: IAU Symposium
- Том: 257
- Год издания: 2009
- Первая страница: 601
- Последняя страница: 603
- DOI: 10.1017/S1743921309029913
- Аннотация: The numerical method developed by Veselovsky & Ivanov (2006), together with magnetograms of the Sun obtained at the photospheric level were used to calculate the coronal magnetic field with open, closed and intermittent topology during March-December 2007. The results of the modelling are compared with stereoscopic images and movies of the corona observed by EUV telescopes onboard STEREO and SOHO spacecraft. The sources of the permanent and transient high speed solar wind streams as well as the sector structure and the heliospheric plasma sheet observed at the Earth's orbit by the ACE and STEREO spacecraft are discussed.
- Добавил в систему: Яковчук Олеся Станиславовна