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On the influence of magnetic topology on the propagation of internal gravity waves in the solar atmosphere
The solar surface is a continuous source of internal gravity waves (IGWs). IGWs are believed to supply the bulk of the wave energy for the lower solar atmosphere, but their existence and role for the energy balance of the upper layers is still unclear, largely due to the lack of knowledge about the...
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| Опубликовано в: : | Philos Trans A Math Phys Eng Sci |
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| Главные авторы: | , , , |
| Формат: | Artigo |
| Язык: | Inglês |
| Опубликовано: |
The Royal Society Publishing
2021
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| Предметы: | |
| Online-ссылка: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7780130/ https://ncbi.nlm.nih.gov/pubmed/33342385 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1098/rsta.2020.0177 |
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