Comparison of Ion–Proton Differential Speed between Interplanetary Coronal Mass Ejections and Solar Wind near 1 au

Comparison of Ion–Proton Differential Speed between Interplanetary Coronal Mass Ejections and Solar Wind near 1 au

The elemental abundance of interplanetary coronal mass ejections (ICMEs) and solar wind near 1 au is often adopted to represent the abundance in the corresponding coronal sources. However, the absolute abundance of heavy ions (relative to hydrogen) near 1 au might be different from the coronal abund...

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Bibliographic Details
Main Authors: Xuechao Zhang, Hongqiang Song, Chengxiao Zhang, Hui Fu, Leping Li, Jinrong Li, Xiaoqian Wang, Rui Wang, Yao Chen
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Solar coronal mass ejections
Solar wind
Solar abundances
Solar cycle
Online Access:https://doi.org/10.3847/1538-4357/ad46f7

Internet

https://doi.org/10.3847/1538-4357/ad46f7

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