On the Relationship Between a Hot-channel-like Solar Magnetic Flux Rope and its embedded Prominence
X. Cheng, M. D. Ding, J. Zhang, A. K. Srivastava, Y. Guo, P. F. Chen, and J. Q. Sun

TL;DR
This study analyzes a solar eruption event, revealing that hot-channel magnetic flux ropes are likely the core structures of eruptions, with kink instability playing a key role in triggering flares and prominence dynamics.
Contribution
It provides observational evidence linking hot-channel flux ropes to magnetic flux ropes and highlights the role of kink instability in solar eruptions.
Findings
Hot-channel and prominence initially cospatial
Kink instability coincides with flare onset
Hot-channel likely the magnetic flux rope system
Abstract
Magnetic flux rope (MFR) is a coherent and helical magnetic field structure that is recently found probably to appear as an elongated hot-channel prior to a solar eruption. In this paper, we investigate the relationship between the hot-channel and associated prominence through analyzing a limb event on 2011 September 12. In the early rise phase, the hot-channel was cospatial with the prominence initially. It then quickly expanded, resulting in a separation of the top of the hot-channel from that of the prominence. Meanwhile, both of them experienced an instantaneous morphology transformation from a shape to a reversed-Y shape and the top of these two structures showed an exponential increase in height. These features are a good indication for the occurrence of the kink instability. Moreover, the onset of the kink instability is found to coincide in time with the impulsive…
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