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Автор Zhang, Jun
Автор Wang, Jingxiu
Автор Nitta, Nariaki
Дата выпуска 2001-02-01
dc.description There are only a few observations published so far that show the initiation of a coronal mass ejection (CME) and illustrate the magnetic changes in the surface origin of a CME. Any attempt to connect a CME with its local solar activities is meaningful. In this paper we present a clear instance of a halo CME initiation. A careful analysis of magnetograms shows that the only obvious magnetic changes in the surface region of the CME is a magnetic flux cancellation underneath a quiescent filament. The early disturbance was seen as the slow upward motion in segments of the quiescent filament. Four hours later, the filament was accelerated to about 50 km s<sup>−1</sup> and erupted. While a small part of the material in the filament was ejected into the upper corona, most of the mass was transported to a nearby region. About forty minutes later, the transported mass was also ejected partially to the upper corona. The eruption of the filament triggered a two-ribbon flare, with post-flare loops connecting the flare ribbons. A halo CME, which is inferred to be associated with the eruptive filament, was observed from LASCO/C2 and C3. The halo CME contained two CME events, each event corresponded to a partial mass ejection of the filament. We suggest that the magnetic reconnection at the lower atmosphere is responsible for the filament eruption and the halo CME.
Формат application.pdf
Издатель Institute of Physics Publishing
Копирайт © 2001 IOP Publishing Ltd
Название A Filament-Associated Halo Coronal Mass Ejection
Тип paper
DOI 10.1088/1009-9271/1/1/85
Print ISSN 1009-9271
Журнал Chinese Journal of Astronomy and Astrophysics
Том 1
Первая страница 85
Последняя страница 98
Аффилиация Zhang, Jun; Beijing Astronomical Observatory, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012
Аффилиация Wang, Jingxiu; Beijing Astronomical Observatory, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012
Аффилиация Nitta, Nariaki; Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA 94304, USA
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