Emerging Near-Surface Solar MHD Dynamos
Using the results of numerical simulations and solar observations, this study shows that the transition from deterministic chaos to hard turbulence in the magnetic field generated by the emerging small-scale, near-surface (within the Sun’s outer 5–10% convection zone) solar MHD dynamos occurs throug...
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| Formato: | Artigo |
| Lenguaje: | Inglês |
| Publicado: |
MDPI AG
2025-09-01
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| Colección: | Foundations |
| Materias: | |
| Acceso en línea: | https://www.mdpi.com/2673-9321/5/3/31 |
| Etiquetas: |
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