Reconnection of a kinking flux rope triggering the ejection of a microwave and hard X-ray source. I. Observations and Interpretation
M. Karlick\'y, B. Kliem

TL;DR
This paper presents observations of a solar flare where a kink instability in a twisted magnetic flux rope leads to reconnection, ejection of sources, and supports the plasmoid interpretation of observed radio and X-ray features.
Contribution
It provides observational evidence linking kink instability to flux rope reconnection and plasmoid formation during a solar flare.
Findings
Evidence of helical kink instability in the flux rope.
Propagation of compact sources at >1000 km/s.
Support for plasmoid interpretation of radio and X-ray sources.
Abstract
Imaging microwave observations of an eruptive, partially occulted solar flare on 18 April 2001 suggest that the global structure of the event can be described by the helical kink instability of a twisted magnetic flux rope. This model is suggested by the inverse gamma shape of the source exhibiting crossing legs of a rising flux loop and by evidence that the legs interact at or near the crossing point. The interaction is reflected by the location of peak brightness near the crossing point and by the formation of superimposed compact nonthermal sources most likely at or near the crossing point. These sources propagate upward along both legs, merge into a single, bright source at the top of the structure, and continue to rise at a velocity ~km\,s. The compact sources trap accelerated electrons which radiate in the radio and hard X-ray ranges. This suggests that they are…
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