Manifestations of three dimensional magnetic reconnection in an eruption of a quiescent filament: \\ Filament strands turning to flare loops
Juraj Lorincik, Jaroslav Dudik, Guillaume Aulanier

TL;DR
This study presents detailed observations of a solar filament eruption where filament strands transformed into flare loops through magnetic reconnection at the ribbon hook, supporting recent 3D flare models.
Contribution
First observational evidence of filament footpoints turning into flare loops via reconnection at the ribbon hook, validating recent 3D flare model predictions.
Findings
Filament strands converted into flare loops during eruption.
Reconnection at the ribbon hook occurred over 150 minutes.
All filament footpoints became flare loop footpoints.
Abstract
We report on observations of conversion of bright filament strands into flare loops during 2012 August 31 filament eruption. Prior to the eruption, individual bright strands composing one of the legs of the filament were observed in the 171 A filter channel data of the Atmospheric Imaging Assembly. After the onset of the eruption, one of the hooked ribbons started to propagate and contract, sweeping footpoints of the bright filament strands as well as coronal loops located close by. Later on, hot flare loops appeared in regions swept by the hook, where the filament strands were rooted. Timing and localization of these phenomena suggest that they are caused by reconnection of field lines composing the filament at the hook, which, to our knowledge, has not been observed before. This process is not included in the standard flare model (CSHKP), as it does not address footpoints of erupting…
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