Linking Magnetic Field Diagnostics with 3D Coronal Mass Ejection Speeds in Solar Active Regions
Understanding how active-region properties influence coronal mass ejection (CME) dynamics is essential for constraining eruption models and improving space-weather prediction. Magnetic diagnostics derived above polarity inversion lines (PILs), including the critical height ( h _crit ) of torus insta...
Enregistré dans:
| Auteurs principaux: | , |
|---|---|
| Format: | Artigo |
| Langue: | Inglês |
| Publié: |
IOP Publishing
2025-01-01
|
| Collection: | The Astrophysical Journal |
| Sujets: | |
| Accès en ligne: | https://doi.org/10.3847/1538-4357/ae1b9f |
| Tags: |
Pas de tags, Soyez le premier à ajouter un tag!
|