Slow Solar Wind: Origin in an Independent Small‐Scale Solar Dynamo
Abstract Separation of the solar wind (SW) into three flow types (coronal mass ejections (CMEs), high speed streams (HSSs), and slow solar wind (SSW)) reveals an inverse relationship between the percentage of time Earth spends in SSW during a year and its annually averaged magnetic field strength (B...
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| Autores principales: | , , |
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| Formato: | Artigo |
| Lenguaje: | Inglês |
| Publicado: |
Wiley
2025-07-01
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| Colección: | Geophysical Research Letters |
| Materias: | |
| Acceso en línea: | https://doi.org/10.1029/2024GL113791 |
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