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Witnessing a Large-scale Slipping Magnetic Reconnection along a Dimming Channel during a Solar Flare View all abstracts by submitter

Ju Jing   Submitted: 2017-06-12 15:24

We report the intriguing large-scale dynamic phenomena associated with the M6.5 flare (SOL2015-06-22T18:23) in NOAA active region 12371, observed by RHESSI, Fermi, and the Atmospheric Image Assembly (AIA) and Magnetic Imager (HMI) on the Solar Dynamic Observatory (SDO). The most interesting feature of this event is a third ribbon (R3) arising in the decay phase, propagating along a dimming channel (seen in EUV passbands) towards a neighboring sunspot. The propagation of R3 occurs in the presence of hard X-ray footpoint emission, and is broadly visible at temperatures from 0.6 MK to over 10 MK through the Differential Emission Measure (DEM) analysis. The coronal loops then undergo an apparent slipping motion following the same path of R3, after a ~80 min delay. To understand the underlying physics, we investigate the magnetic configuration and the thermal structure of the flaring region. Our results are in favor of a slipping-type reconnection followed by the thermodynamic evolution of coronal loops. In comparison with those previously reported slipping reconnection events, this one proceeds across a particularly long distance (~60 Mm) over a long period of time (~50 min), and shows two clearly distinguished phases: the propagation of the footpoint brightening driven by nonthermal particle injection and the apparent slippage of loops governed by plasma heating and subsequent cooling.

Authors: Ju Jing, Rui Liu, Mark C. M. Cheung, Jeongwoo Lee, Yan Xu, Chang Liu, Chunming Zhu, and Haimin Wang
Projects: Fermi/GBM,RHESSI,SDO-AIA,SDO-HMI

Publication Status: accepted for publication in ApJL
Last Modified: 2017-06-14 10:02
Go to main E-Print page  Detection and Interpretation Of Long-Lived X-Ray Quasi-Periodic   Pulsations in the X-Class Solar Flare On 2013 May 14  Investigation of Relationship Between High-Energy X-ray Sources and Photospheric and Helioseismic Impacts of X1.8 Solar Flare of October 23, 2012  Edit Entry  Download Preprint  Delete Entry 

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