Variations of Heavy Ions in Interplanetary Shock Driven by Interplanetary Coronal Mass Ejections and Stream Interaction Regions

Variations of Heavy Ions in Interplanetary Shock Driven by Interplanetary Coronal Mass Ejections and Stream Interaction Regions

In the solar wind, the fluctuation of heavy ion abundance serves as a crucial physical metric. This not only mirrors the attributes of the solar wind’s originating solar region but also signifies its influence on Earth’s magnetosphere. Utilizing data from the Advanced Composition Explorer satellite,...

Full description

Bibliographic Details
Main Authors: Cong Wang, Qian Ye, Mu Li, Fei He, Xiaoxin Zhang
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal Supplement Series
Subjects:
Solar coronal mass ejection shocks
Solar wind
Abundance ratios
Corotating streams
Online Access:https://doi.org/10.3847/1538-4365/ad2fb2

Internet

https://doi.org/10.3847/1538-4365/ad2fb2

Similar Items