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Successive Coronal Jets as Novel Facilitators for Filament Oscillation and Eruption

  • Authors: Chengrui Zhou, Chun Xia, Wentai Fu, Hechao Chen, Qiaoling Li

Chengrui Zhou et al 2026 The Astrophysical Journal Letters 1006 .

  • Provider: AAS Journals

Caption: Figure 6.

Panels (a1)–(a7) present Hinode/XRT soft X-ray images (Al-poly filter). Panel (b) shows the soft X-ray light curve integrated over the FOV of (a1)–(a7); the yellow and blue stars indicate the two exposure modes of XRT (long and short, respectively). Panels (c) and (d) display the 2D magnetic field lines in the central xz cross section from the simulation. Panel (e) shows the electric field Ey along the CS during the filament eruption; the red stars mark the timing of the jets in the simulation, and the filament height is derived from the center of the simulated flux rope.

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