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Can We Distinguish the Source Region Location of Filament/Prominence Eruptions from the Sun-as-a-star Hα Spectrum?

  • Authors: Junyi Zhang, Yijun Hou, Xiaofeng Liu, Ting Li, Shihao Rao, Ye Qiu, HuiPing Jin, Yingjie Cai, Yangrui Chen, Chuan Li

Junyi Zhang et al 2026 The Astrophysical Journal 1004 .

  • Provider: AAS Journals

Caption: Figure 2.

CHASE imaging and spectral observations of the event occurred on 2024 June 10 (event 3, farside limb active region eruption). (a)–(e) The same as Figures 1(a1)–(e1) but for event 3. (b1) and (b2) and (d1) and (d2) indicate different observation time. The navy and gray arrows mark the erupting materials and postflare loops. An animation is available online, which displays the evolution of event 3. The animation’s duration is 2 s.

(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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