The Formation of a Bulge at the Front of Solar Coronal Mass Ejections
Coronal mass ejections (CMEs) are associated with eruptions of magnetic flux ropes (MFRs). Recent studies have proposed a new explanation on the nature of the three-part structure of CMEs, in which the front results from plasma pileup along the overlying coronal loops and should exhibit a smooth arc...
Wedi'i Gadw mewn:
| Prif Awduron: | , , , , , , , , |
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| Fformat: | Artigo |
| Iaith: | Inglês |
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IOP Publishing
2026-01-01
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| Cyfres: | The Astrophysical Journal |
| Pynciau: | |
| Mynediad Ar-lein: | https://doi.org/10.3847/1538-4357/ae61aa |
| Tagiau: |
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