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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 5.

Solar wind plasma and magnetic field parameters detected at Wind (a) and STEREO-A (b) spacecraft. (a) From top to bottom, the panels show the proton density, bulk speed, proton temperature (the dotted curve denotes the expected proton temperature from the observed speed), magnetic field strength, proton β, magnetic field components, and Dst index. (b) Same as (a), but without the Dst index. The yellow and blue shaded regions indicate the intervals of the two ejecta, and the blue vertical dashed lines mark the associated shocks.

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