A complicated solar eruption event on 2003 October 26 |
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Authors: | Zongjun Ning M. D. Ding K. P. Qiu H. Li Y. N. Su C. Fang |
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Affiliation: | 1. Purple Mountain Observatory, Nanjing, 210008, China 2. Department of Astronomy, Nanjing University, Nanjing, 210093, China
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Abstract: | We present multi-wavelength observations of a complicated solar eruption event to associate with an X1.2 flare and a Coronal Mass Ejection (CME) on 2003 October 26. The soft X-ray profile shows a possibility for occurrence of two flares with peaks around 06:20 and 07:00 UT. According to our observations, there are many evidences to show that they are corresponding to two energy releases. The first one produces type II, type III, moving type IV continua, a decimetric burst (DCIM) and strong emissions at Hα, 195 and 1600 Å; While the second energy release only produces a group of RS-III bursts, DCIM and Hα emissions. It appears that the first energy release is associated with a CME, while the second CME is quiet. Such observational difference between two energy releases is found indicating two magnetic reconnection processes occurrence with different plasma situation. |
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