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High-resolution wave dynamics in the lower solar atmosphere
The magnetic and convective nature of the Sun’s photosphere provides a unique platform from which generated waves can be modelled, observed and interpreted across a wide breadth of spatial and temporal scales. As oscillations are generated in-situ or emerge through the photospheric layers, the inter...
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| Publicado en: | Philos Trans A Math Phys Eng Sci |
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| Main Authors: | , , , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado: |
The Royal Society Publishing
2021
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| Assuntos: | |
| Acceso en liña: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7780137/ https://ncbi.nlm.nih.gov/pubmed/33342388 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1098/rsta.2020.0169 |
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