How flux feeding causes eruptions of solar magnetic flux ropes with the hyperbolic flux tube configuration?
Quanhao Zhang, Rui Liu, Yuming Wang, Zhenjun Zhou, Bin Zhuang, Xiaolei, Li

TL;DR
This study uses a 2.5D MHD model to investigate how flux feeding influences the eruption of solar magnetic flux ropes with hyperbolic flux tube configurations, revealing that flux feeding can both trigger and stabilize eruptions depending on flux injection.
Contribution
It demonstrates that flux feeding can induce eruptions in HFT-configured flux ropes by injecting axial flux, expanding understanding of eruption mechanisms beyond previous bald patch models.
Findings
Flux feeding injects axial magnetic flux into the flux rope.
Flux feeding can trigger eruptions if enough axial flux is injected.
Flux feeding can stabilize flux ropes if the injected flux is insufficient.
Abstract
Coronal magnetic flux ropes are generally considered to be the core structure of large-scale solar eruptions. Recent observations found that solar eruptions could be initiated by a sequence of "flux feeding," during which chromospheric fibrils rise upward from below, and merge with a pre-existing prominence. Further theoretical study has confirmed that the flux feeding mechanism is efficient in causing the eruption of flux ropes that are wrapped by bald patch separatrix surfaces. But it is unclear how flux feeding influences coronal flux ropes that are wrapped by hyperbolic flux tubes (HFT), and whether it is able to cause the flux-rope eruption. In this paper, we use a 2.5-dimensional magnetohydrodynamic model to simulate the flux feeding processes in HFT configurations. It is found that flux feeding injects axial magnetic flux into the flux rope, whereas the poloidal flux of the rope…
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