The quiet sun at mm wavelengths as seen by ALMA
Solar observations at sub-mm, mm and cm wavelengths offer a straightforward diagnostic of physical conditions in the solar atmosphere because they yield measurement of brightness temperature which, for optically thick features, equals intrinsic temperature - much unlike solar diagnostics in other sp...
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| Autors principals: | , , |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Frontiers Media S.A.
2022-10-01
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| Col·lecció: | Frontiers in Astronomy and Space Sciences |
| Matèries: | |
| Accés en línia: | https://www.frontiersin.org/articles/10.3389/fspas.2022.981320/full |
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