Simulating high-speed solar wind streams from coronal holes using an L5-L1 configuration of Lagrangian points

Simulating high-speed solar wind streams from coronal holes using an L5-L1 configuration of Lagrangian points

Abstract Coronal holes (CHs) are known to be sources of high-speed solar wind streams (HSSs), yet the physical mechanisms linking CH position and characteristics to solar wind (SW) behaviour remain unclear. Our results reveal that the latitude of CHs, especially smaller ones, combined with the helio...

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Bibliographic Details
Main Authors: Tatiana Podladchikova, Astrid M. Veronig, Manuela Temmer, Stefan J. Hofmeister
Format: Article
Language:English
Published: Nature Portfolio 2025-04-01
Series:Scientific Reports
Subjects:
The Sun
Solar coronal holes
Fast solar wind
Lagrangian points
Solar physics
Online Access:https://doi.org/10.1038/s41598-025-97246-2
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https://doi.org/10.1038/s41598-025-97246-2

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