Formation and Evolution of Transient Prominence Bubbles Driven by Erupting Minifilaments
Prominence bubbles, the dark arch-shaped voids below quiescent prominences, are generally believed to be caused by the interaction between the prominences and the slowly emerging or quasi-stable underlying magnetic loops. However, this scenario could not explain some short-lived bubbles with extreme...
Sábháilte in:
| Príomhchruthaitheoirí: | , , , , , , , , |
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| Formáid: | Artigo |
| Teanga: | Inglês |
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IOP Publishing
2024-01-01
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| Sraith: | The Astrophysical Journal |
| Ábhair: | |
| Rochtain ar líne: | https://doi.org/10.3847/1538-4357/ad54b8 |
| Clibeanna: |
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