Magnetorotational Instability in a Solar Near-surface Mean-field Dynamo
We address the question whether the magnetorotational instability (MRI) can operate in the near-surface shear layer (NSSL) of the Sun and how it affects the interaction with the dynamo process. Using hydromagnetic mean-field simulations of α Ω-type dynamos in rotating shearing-periodic boxes, we sho...
-д хадгалсан:
| Үндсэн зохиолчид: | , , , |
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| Формат: | Artigo |
| Хэл сонгох: | Inglês |
| Хэвлэсэн: |
IOP Publishing
2025-01-01
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| Цуврал: | The Astrophysical Journal |
| Нөхцлүүд: | |
| Онлайн хандалт: | https://doi.org/10.3847/1538-4357/ae03c4 |
| Шошгууд: |
Шошго байхгүй, Энэхүү баримтыг шошголох эхний хүн болох!
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