Long-duration Nonthermal Motions in the Supra-arcade and Loop-top Region during an Eruptive Solar Flare
Solar flares are widely accepted to be powered by magnetic reconnection that involves complex dynamics in various scales. The flare supra-arcade and loop-top region, directly impacted by fast reconnection downflows, contains a wealth of microscopic dynamics, which are, however, difficult to resolve...
-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/addd20 |
| Шошгууд: |
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