Magnetic structure of coronal dark halos
Context. At low coronal temperatures around or below 1 MK distinct areas in the surroundings of active regions (ARs) show emission at a level significantly below the emission coming from the quiet Sun (QS). These areas are referred to as dark halos, dark canopies, or dark moats. Aims. To better unde...
Gorde:
| Egile Nagusiak: | , , , , , , , |
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| Formatua: | Artigo |
| Hizkuntza: | Inglês |
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EDP Sciences
2026-05-01
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| Saila: | Astronomy & Astrophysics |
| Gaiak: | |
| Sarrera elektronikoa: | https://www.aanda.org/articles/aa/full_html/2026/05/aa57009-25/aa57009-25.html |
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