Breakout and Tether-cutting Eruption Models Are Both Catastrophic (Sometimes)
arXiv:1312.4435 · doi:10.1007/s11207-013-0464-8
Abstract
We present a simplified analytic model of a quadrupolar magnetic field and flux rope to model coronal mass ejections. The model magnetic field is two-dimensional, force-free and has current only on the axis of the flux rope and within two currents sheets. It is a generalization of previous models containing a single current sheet anchored to a bipolar flux distribution. Our new model can undergo quasi-static evolution due either to changes at the boundary or to magnetic reconnection at either current sheet. We find that all three kinds of evolution can lead to a catastrophe known as loss of equilibrium. Some equilibria can be driven to catastrophic instability either through reconnection at the lower current sheet, known as tether cutting, or through reconnection at the upper current sheet, known as breakout. Other equilibria can be destabilized through only one and not the other. Still others undergo no instability, but evolve increasingly rapidly in response to slow steady driving (ideal or reconnective). One key feature of every case is a response to reconnection different from that found in simpler systems. In our two-current sheet model a reconnection electric field in one current sheet causes the current in that sheet to {\em increase} rather than decrease. This suggests the possibility for the microscopic reconnection mechanism to run away.
References in corpus (2)
Cited by in corpus (19)
- Flare-productive active regions
- Magnetic reconnection in the era of exascale computing and multiscale experiments
- Catastrophe versus instability for the eruption of a toroidal solar magnetic flux rope
- Flux-Rope Twist in Eruptive Flares and CMEs: due to Zipper and Main-Phase Reconnection
- Probing the Physics of the Solar Atmosphere with the Multi-slit Solar Explorer (MUSE): II. Flares and Eruptions
- Structure and Evolution of Magnetic Fields Associated with Solar Eruptions (Invited Review)
- Solar Magnetic Flux Ropes
- Unwinding motion of a twisted active-region filament
- Flux Accretion and Coronal Mass Ejection Dynamics
- Failed prominence eruptions near 24 cycle maximum
- Eruption of Solar Magnetic Flux Ropes Caused by Flux Feeding
- Two-step solar filament eruptions
- Downward catastrophe of solar magnetic flux ropes
- Influence of photospheric magnetic conditions on the catastrophic behaviors of flux ropes in active regions
- Confined and eruptive catastrophes of solar magnetic flux ropes caused by mass loading and unloading
- Tracing Field Lines That Are Reconnecting or Expanding or Both
- Upward and downward catastrophes of coronal magnetic flux ropes in quadrupolar magnetic fields
- How flux feeding causes eruptions of solar magnetic flux ropes with the hyperbolic flux tube configuration?
- Energy Build-up and Triggering Leading to a M1.5 Flare on 1 August 2014