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Mystery behind the Peeling of a Filament and the Associated Sudden Disappearance of a Sunspot Penumbra

  • Authors: Ju Jing, Mia Mancuso, Satoshi Inoue, Jeongwoo Lee, Qin Li, Wen He, Yan Xu, Wenda Cao, Haimin Wang

Ju Jing et al 2025 The Astrophysical Journal Letters 993 .

  • Provider: AAS Journals

Caption: Figure 6.

The evolution of penumbral horizontal and vertical field strength in the simulation. Left: HMI Bz map at 17:00 UT, showing the FOV of the bottom boundary of the NLFFF model and the simulation. The box indicates the region of penumbra disappearance, which is the same as the region shown by the box in Figure 3(f). Right: time profiles of ∣Bh∣ (solid) and ∣Bz∣ (dotted), averaged over the boxed region shown in the left panel. The simulation time “0” corresponds to 17:00 UT.

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