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Weak influence of near-surface layer on solar deep convection zone revealed by comprehensive simulation from base to surface
The solar convection zone is filled with turbulent convection in highly stratified plasma. Several theoretical and observational studies suggest that the numerical calculations overestimate the convection velocity. Since all deep convection zone calculations exclude the solar surface due to substant...
| Autores principales: | , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
American Association for the Advancement of Science
2019
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| Materias: | |
| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6314832/ https://www.ncbi.nlm.nih.gov/pubmed/30613769 http://dx.doi.org/10.1126/sciadv.aau2307 |