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Dark Ribbons Propagating and Sweeping Across EUV Structures After Filament Eruptions View all abstracts by submitter

Ting Li   Submitted: 2015-05-17 21:06

With observations from the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory, we first report that dark ribbons (DRs) moved apart from the filament channel and swept across EUV structures after filament eruptions on 2013 June 23 and 2012 February 10 and 24, respectively. In the first event, the DR with a length of 168Mm appeared at 100Mm to the northwest of the filament channel, where the filament erupted 15 hr previously. The DR moved toward the northwest with the different sections having different velocities, ranging from 0.3 to 1.6 km s-1. When the DR?s middle part swept across a strong EUV structure, the motion of this part was blocked, appearing to deflect the DR. With the DR propagation, the connection of the surrounding EUV structures gradually changed. After one day passed, the DR eventually disappeared. In the other two events, the dynamic evolution of the DRs was similar to that in the first event. Based on the observations, we speculate that the reconnection during the filament eruption changes the configuration of the surrounding magnetic fields systematically. During the reconnection process, magnetic fields are deflecting and the former arbitrarily distributed magnetic fields are rearranged along specific directions. The deflection of magnetic fields results in an instantaneous void region where the magnetic strength is smaller and the plasma density is lower. Consequently, the void region is observed as a DR and propagates outward with the reconnection developing.

Authors: Junmin Xiao, Jun Zhang, Ting Li, and Shuhong Yang
Projects: SDO-AIA

Publication Status: published online, ApJ,805,25
Last Modified: 2015-05-19 08:51
Go to main E-Print page  SunPy - Python for Solar Physics  Forward Modelling of standing slow modes of flaring coronal loops  Edit Entry  Download Preprint  Delete Entry 

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