Characteristics and Source Regions of Slow Alfvénic Solar Wind Observed by Parker Solar Probe

Characteristics and Source Regions of Slow Alfvénic Solar Wind Observed by Parker Solar Probe

Using a classification scheme for solar-wind type based on the heliocentric distance of the observation, we look at near-perihelion observations from Parker Solar Probe Encounters 4 to 14 to study the sources of the slow Alfvénic solar wind (SASW). Through Potential Field Source Surface (PFSS) model...

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Bibliographic Details
Main Authors: Tamar Ervin, Kai Jaffarove, Samuel T. Badman, Jia Huang, Yeimy J. Rivera, Stuart D. Bale
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Slow solar wind
Solar magnetic fields
Solar coronal holes
Online Access:https://doi.org/10.3847/1538-4357/ad7d00
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