A Model for Energy Buildup and Eruption Onset in Coronal Mass Ejections

@article{Dahlin2019AMF,
  title={A Model for Energy Buildup and Eruption Onset in Coronal Mass Ejections},
  author={Joel T. Dahlin and Spiro K. Antiochos and C. Richard DeVore},
  journal={The Astrophysical Journal},
  year={2019}
}
Coronal mass ejections (CMEs) and eruptive flares (EFs) are the most energetic explosions in the solar system. Their underlying origin is the free energy that builds up slowly in the sheared magnetic field of a filament channel. We report the first end-to-end numerical simulation of a CME/EF, from zero-free-energy initial state through filament-channel formation to violent eruption, driven solely by the magnetic-helicity condensation process. Helicity is the topological measure of linkages… 

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