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Turbulence in the Sun is suppressed on large scales and confined to equatorial regions
Convection in the Sun’s outer envelope generates turbulence and drives differential rotation, meridional circulation, and the global magnetic cycle. We develop a greater understanding of these processes by contrasting observations with simulations of global convection. These comparisons also enhance...
| Autores principales: | , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
American Association for the Advancement of Science
2020
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| Materias: | |
| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7450475/ https://www.ncbi.nlm.nih.gov/pubmed/32923604 http://dx.doi.org/10.1126/sciadv.aba9639 |