Reconnection in explosive phenomena
Determine how and under what conditions magnetic reconnection acts as a driver or consequence of explosive phenomena, establish whether solar eruptions are triggered by torus instability, kink instability, or both, and characterize reconnection’s contribution to those eruptions.
References
However, without detailed modelling, we cannot determine whether both sources were produced by external reconnection or whether one was related to reconnection underneath the flux rope.
Explosive phenomena problem: How, and under what conditions, does magnetic reconnection act either as a driver or a consequence of explosive phenomena such as solar flares, Coronal Mass Ejections, and disruptive phenomena in fusion plasmas? Are solar eruptions triggered by torus instability, kink instability, or a combination of both? How does reconnection contribute to these eruptions?
The internal eruption appears to commence prior to the brightenings of the outer footpoint sources, likely supporting the tether-cutting model \citep{2006GMS...165...43M}. However, it should be noted that we cannot rule out the possibility that the eruption was triggered by ideal MHD instabilities or a loss of equilibrium.
Whether this process genuinely constitutes an avalanche-like chain reaction, or whether the sequential brightenings are independently driven by a common external trigger such as progressive photospheric shearing and flux emergence, remains an open question.