Chromospheric Magnetic Field Extrapolations Reveal the Flux-rope Configuration of a Solar Filament
Solar eruptions are powered by the release of magnetic energy stored in the lower solar atmosphere, but the preeruptive magnetic configuration of filament channels remains difficult to determine. A central question is whether this energy is stored in a preexisting magnetic flux rope or in a sheared...
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| Principais autores: | , , , , , , , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
IOP Publishing
2026-01-01
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| Colecção: | The Astrophysical Journal Letters |
| Assuntos: | |
| Acesso em linha: | https://doi.org/10.3847/2041-8213/ae9873 |
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