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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 3.

Computed DEM results. (a)–(d) Temporal evolution of the DEM-weighted temperature distribution. The dark blue arrows point to the drifting end of the northern heated loops. (e)–(f) DEM images at 02:19:59 UT showing the coronal plasma in the temperature ranges of 1.0–1.5 MK and 8.0–11.0 MK, respectively.

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