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...
I tiakina i:
| Ngā kaituhi matua: | , , , , , |
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| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
EDP Sciences
2026-04-01
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| Rangatū: | Astronomy & Astrophysics |
| Ngā marau: | |
| Urunga tuihono: | https://www.aanda.org/articles/aa/full_html/2026/04/aa59286-26/aa59286-26.html |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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