Dynamics, thermodynamics, and fine structure of virtual erupting filaments
Context. It is not fully understood why some solar filaments erupt, whereas others do not. Filaments that erupt typically undergo a slow rise, followed by an acceleration phase; this transition requires further investigation. Erupting prominences have been observed to heat up during the acceleration...
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| Hlavní autoři: | , , , |
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| Médium: | Artigo |
| Jazyk: | Inglês |
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EDP Sciences
2026-03-01
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| Edice: | Astronomy & Astrophysics |
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| On-line přístup: | https://www.aanda.org/articles/aa/full_html/2026/03/aa57941-25/aa57941-25.html |
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