Sympathetic Quiet and Active Region Filament Eruptions

Kostadinka Koleva; Pooja Devi; Ramesh Chandra; Reetika Joshi; Peter Duchlev; Momchil Dechev

doi:10.1007/s11207-022-01981-y

Sympathetic Quiet and Active Region Filament Eruptions

Solar and Stellar Astrophysics 2022-04-20 v1

Authors: Kostadinka Koleva , Pooja Devi , Ramesh Chandra , Reetika Joshi , Peter Duchlev , Momchil Dechev

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Abstract

We present the observations of three sympathetic filament eruptions occurring on 19 July 2015 namely F1, F2, and F3. The events were observed in UV/EUV wavelengths by Atmospheric Imaging Assembly onboard the Solar Dynamics Observatory and by Global Oscillation Network Group telescope in H{\alpha} line. As filament F1 starts to erupt, a part of it falls close to the location of the F2 and F3 filaments. This causes the eruption of F2 and F3 during which the two filaments merge together and trigger a medium-class CME and a long-duration GOES C2.1 class flare. We discuss the dynamics and kinematics of these three filament eruptions and related phenomena.

Keywords

sympathetic eruptions solar filaments coronal mass ejection solar flare sdo/aia h-alpha

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@article{arxiv.2202.08157,
  title  = {Sympathetic Quiet and Active Region Filament Eruptions},
  author = {Kostadinka Koleva and Pooja Devi and Ramesh Chandra and Reetika Joshi and Peter Duchlev and Momchil Dechev},
  journal= {arXiv preprint arXiv:2202.08157},
  year   = {2022}
}

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19 pages, 12 Figures

Sympathetic Quiet and Active Region Filament Eruptions

Abstract

Keywords

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