A complicated solar eruption event on 2003 October 26. Solar flare
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 H α, 195 and 1600 Å; While the second energy release only produces a group of RS-III bursts, DCIM and H α 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.
- Publication:
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Astrophysics and Space Science
- Pub Date:
- June 2008
- DOI:
- 10.1007/s10509-008-9790-y
- Bibcode:
- 2008Ap&SS.315...45N
- Keywords:
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- Sun: flares;
- Sun: radio radiation