English

Interaction of Two Filament Channels of Different Chiralities

Solar and Stellar Astrophysics 2016-07-20 v1

Abstract

We present observations of interactions between the two filament channels of different chiralities and associated dynamics that occurred during 2014 April 18 -- 20. While two flux ropes of different helicity with parallel axial magnetic fields can only undergo a bounce interaction when they are brought together, the observations at the first glance show that the heated plasma is moving from one filament channel to the other. The SDO/AIA 171 A observations and the PFSS magnetic field extrapolation reveal the presence of fan-spine magnetic configuration over the filament channels with a null point located above them. Three different events of filament activations, partial eruptions, and associated filament channel interactions have been observed. The activation initiated in one filament channel seems to propagate along the neighbour filament channel. We believe that the activation and partial eruption of the filaments bring the field lines of flux ropes containing them closer to the null point and trigger the magnetic reconnection between them and the fan-spine magnetic configuration. As a result, the hot plasma moves along the outer spine line toward the remote point. Utilizing the present observations, for the first time we have discussed how two different-chirality filament channels can interact and show interrelation.

Keywords

Cite

@article{arxiv.1605.01812,
  title  = {Interaction of Two Filament Channels of Different Chiralities},
  author = {Navin Chandra Joshi and Boris Filippov and Brigitte Schmieder and Tetsuya Magara and Young-Jae Moon and Wahab Uddin},
  journal= {arXiv preprint arXiv:1605.01812},
  year   = {2016}
}

Comments

30 pages, 13 figures, Accepted for Publication in ApJ