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Flareless enhancement of solar energetic particle flux on April 14-17, 1994статья
Информация о цитировании статьи получена из
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Статья опубликована в журнале из списка Web of Science и/или Scopus
Дата последнего поиска статьи во внешних источниках: 28 мая 2015 г.
- Авторы: Veselovsky I.S., Gotselyuk Yu V., Dmitriev A.V., Kuznetsov S.N., Kurt V.G., Myagkova I.N., Oraevsky V.N., Panasyuk M.I., Podorolsky A.N., Ryumin S.P.
- Журнал: Cosmic Research (English translation of Kosimicheskie Issledovaniya)
- Том: 35
- Номер: 2
- Год издания: 1997
- Издательство: Pleiades Publishing, Inc.
- Местоположение издательства: New York, USA
- Первая страница: 119
- Последняя страница: 124
- Аннотация: The solar cosmic ray event of April 14-17, 1994, with energies of protons E p > 30 MeV and electrons E e > 1.3 MeV observed aboard the CORONAS-I satellite over Earth’s polar caps, is discussed. This event is not associated with any impulsive solar flare nor with any active region. This suggests that the observed event is a flareless particle flux increase. Features of particle propagation in interplanetary space are discussed. We assume that in this case, acceleration of solar energetic particles is related to an eruptive event observed by the SXT instrument aboard the Yohkoh satellite. This Solar Particle Crown event is one of the most large-scale dynamical events in the soft X-ray range recorded aboard the satellite. The relationship between the coronal and interplanetary signatures of this phenomenon is important in many respects. В© 1997 MAEe Cyrillic signK HayОєa/Interperiodica Publishing.
- Добавил в систему: Мягкова Ирина Николаевна