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A Major Geomagnetic Storm in 2024 October Linked to Sympathetic Coronal Mass Ejection–Prominence Eruptions

  • Authors: Rui Wang, Huidong Hu, Xiaowei Zhao, Chong Chen, Suli Ma, Zhongwei Yang, Lei Lu, Li Feng, Wenshuai Cheng, Chong Huang, Quan Wang, Xiaoshuai Zhu, Bei Zhu, Yiming Jiao

Rui Wang et al 2026 The Astrophysical Journal Letters 1002 .

  • Provider: AAS Journals

Caption: Figure 3.

Evolution of two CMEs observed by coronagraphs on October 9. (a) and (b) Running-difference (RD) white-light images observed by ASO-S/SCIWL. Red and blue arrows indicate CME1 (QF-CME) and CME2 (AR-CME), respectively. (c) Composite RD images of SCIWL and LASCO/C2. Red and blue dotted lines outline the leading edges of two CMEs. (d) and (e) GCS wireframes overplotted on SCIWL and STEREO-A/COR1. Blue (red) wireframe corresponds to AR-CME (QF-CME). (f) and (g) GCS modeling from C2 and STEREO-A/COR2. The green arrows indicate two distinct shocks. (h) and (i) Spheroid shock modeling (golden) from LASCO/C3 and COR2. An animation of panels (a) and (b) shows two CMEs with distinct leading edges propagating outwards in the SCIWL from 01:57 to 02:55 UT (2 s duration).

(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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