Multiple magnetic reconnection sites associated with a coronal mass ejection in the solar wind
نویسندگان
چکیده
منابع مشابه
Multi-wavelength Signatures of Magnetic Reconnection of a Flare Associated Coronal Mass Ejection
The evolution of an X2.7 solar flare, that occurred in a complex βγδ magnetic configuration region on 2003 November 3, is discussed utilizing a multiwavelength data set. The Hα images taken from the solar tower telescope at ARIES, Nainital, reveal well-defined footpoint (FP) and loop-top (LT) sources. As the flare evolves, the LT source moves upward and the separation between the two FP sources...
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The driving mechanism of solar flares and coronal mass ejections is a topic of ongoing debate, apart from the consensus that magnetic reconnection plays a key role during the impulsive process. While present solar research mostly depends on observations and theoretical models, laboratory experiments based on high-energy density facilities provide the third method for quantitatively comparing as...
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ژورنال
عنوان ژورنال: Journal of Geophysical Research: Space Physics
سال: 2007
ISSN: 0148-0227
DOI: 10.1029/2007ja012418