Chromospheric and photospheric properties of sunspots as inferred from Stokes inversions under magnetohydrostatic and non-local thermodynamic equilibrium
Context. Sunspots represent a key feature in the solar atmosphere to explore how magnetic fields interact with plasma flows, exhibiting large variations in physical parameters over very small spatial scales (< 100 km), and sometimes featuring dynamic phenomena such as oscillatory umbral flashes. To...
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| Principais autores: | , , , , , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado: |
EDP Sciences
2026-04-01
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| Series: | Astronomy & Astrophysics |
| Assuntos: | |
| Acceso en liña: | https://www.aanda.org/articles/aa/full_html/2026/04/aa59286-26/aa59286-26.html |
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