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Evolution of Magnetic Flux Rope and Its Overlying Arcade Based on Nonlinear Force-free Field Extrapolations View all abstracts by submitter

Ju Jing   Submitted: 2014-03-11 09:17

Dynamic phenomena indicative of slipping reconnection and magnetic implosion were found in a time series of nonlinear force-free field (NLFFF) extrapolations for the active region 11515, which underwent significant changes in the photospheric fields and produced five C-class flares and one M-class flare over five hours on 2012 July 2. NLFFF extrapolation was performed for the uninterrupted 5 hour period from the 12 minute cadence vector magnetograms of the Helioseismic and Magnetic Imager on board the Solar Dynamic Observatory. According to the time-dependent NLFFF model, there was an elongated, highly sheared magnetic flux rope structure that aligns well with an Hα filament. This long filament splits sideways into two shorter segments, which further separate from each other over time at a speed of 1-4 km s-1, much faster than that of the footpoint motion of the magnetic field. During the separation, the magnetic arcade arching over the initial flux rope significantly decreases in height from ~4.5 Mm to less than 0.5 Mm. We discuss the reality of this modeled magnetic restructuring by relating it to the observations of the magnetic cancellation, flares, a filament eruption, a penumbra formation, and magnetic flows around the magnetic polarity inversion line.

Authors: Ju Jing, Chang Liu, Jeongwoo Lee, Shuo Wang, Thomas Wiegelmann, Yan Xu, and Haimin Wang
Projects: SDO-HMI

Publication Status: ApJ, 784, L13
Last Modified: 2014-03-12 09:55
Go to main E-Print page  Thermal structure of hot non-flaring corona from Hinode/EIS  Two Sun-like Superflare Stars Rotating as Slow as the Sun  Edit Entry  Download Preprint  Delete Entry 

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