Coronal mass ejection precursors in Sun-like stars: Flux rope modelling and coronal signatures
Context. Coronal mass ejections (CMEs) are among the most energetic manifestations of solar and stellar activity. In the Sun, they play a central role in space weather, while in more active stars, the solar paradigm indicates that they should be even more frequent and energetic. However, many CMEs p...
Wedi'i Gadw mewn:
| Prif Awduron: | , , , |
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| Fformat: | Artigo |
| Iaith: | Inglês |
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EDP Sciences
2026-05-01
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| Cyfres: | Astronomy & Astrophysics |
| Pynciau: | |
| Mynediad Ar-lein: | https://www.aanda.org/articles/aa/full_html/2026/05/aa58021-25/aa58021-25.html |
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