Classification of Enhanced Geoeffectiveness Resulting from High-speed Solar Wind Streams Compressing Slower Interplanetary Coronal Mass Ejections

Classification of Enhanced Geoeffectiveness Resulting from High-speed Solar Wind Streams Compressing Slower Interplanetary Coronal Mass Ejections

High-speed solar wind streams (HSSs) interact with the preceding ambient solar wind to form stream interaction regions (SIRs), which are a primary source of recurrent geomagnetic storms. However, HSSs may also encounter and subsequently interact with interplanetary coronal mass ejections (ICMEs). In...

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Bibliographic Details
Main Authors: Stephan G. Heinemann, Chaitanya Sishtla, Simon Good, Maxime Grandin, Jens Pomoell
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal Letters
Subjects:
The Sun
Solar coronal mass ejections
Solar wind
Fast solar wind
Solar-terrestrial interactions
Space weather
Online Access:https://doi.org/10.3847/2041-8213/ad283a

Internet

https://doi.org/10.3847/2041-8213/ad283a

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