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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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| Udgivet i: | Philos Trans A Math Phys Eng Sci |
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| Main Authors: | , , , |
| Format: | Artigo |
| Sprog: | Inglês |
| Udgivet: |
The Royal Society Publishing
2021
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| Fag: | |
| Online adgang: | 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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