Similarities and Differences between ICME-driven Shocks Observed by VEX (∼0.72 au) and WIND (∼1.0 au)

Similarities and Differences between ICME-driven Shocks Observed by VEX (∼0.72 au) and WIND (∼1.0 au)

The features of interplanetary shocks driven by interplanetary coronal mass ejections (ICMEs) observed by WIND (∼1.0 au) and Venus Express (VEX; ∼0.72 au) during the same period are statistically analyzed by comparing their similarities and differences. It is found that the proportion of ICME-driven...

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Bibliographic Details
Main Authors: Mengsi Ruan, Pingbing Zuo, Zilu Zhou, Jiayun Wei, Xueshang Feng, Yi Wang, Qi Xu, Xiaojun Xu, Zhengyang Zou, Zhenning Shen
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Interplanetary shocks
Astronomy data analysis
Solar coronal mass ejections
Interplanetary magnetic fields
Online Access:https://doi.org/10.3847/1538-4357/ada35b
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https://doi.org/10.3847/1538-4357/ada35b

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