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Self-constrained Magnetic Reconnection of a Solar Flare Cospatial with a Nonejected Filament

  • Authors: Ye Qiu, Changxue Chen, Anqin Chen, Chuan Li, Yang Guo, Linggao Kong, Feng Lu, Xiaohu Zhang, Weiguo Zong, Jinsong Wang, Xinkai Li, Peng Wang, Kefei Song, Bo Chen

Ye Qiu et al 2026 The Astrophysical Journal Letters 1010 .

  • Provider: AAS Journals

Caption: Figure 2.

SDO/AIA EUV observations of the nonejected central filament, and the ejection of the eastern small filament disturbed by the nearby C6.1 flare. (a)–(d) 304 Å images at four selected times. The blue arrows point to the eastern small filament. (e)–(f) 94 Å images before the flare and at its onset, respectively. (g)–(h) 171 Å running-difference images showing the ejection of the small filament. The white arrows in (g) outline the leading-edge structure of the filament ejection. A 19 s animation is available, showing the evolution of the flare and the ejection of the small filament in SDO/AIA 304 Å images and 171 Å running-difference images.

(An animation of this figure is available in the online article.)

(An animation of this figure is available.)

The video/animation of this figure is available in the online journal.

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