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Deep rotating convection generates the polar hexagon on Saturn
Numerous land- and space-based observations have established that Saturn has a persistent hexagonal flow pattern near its north pole. While observations abound, the physics behind its formation is still uncertain. Although several phenomenological models have been able to reproduce this feature, a s...
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| Wydane w: | Proc Natl Acad Sci U S A |
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| Główni autorzy: | , |
| Format: | Artigo |
| Język: | Inglês |
| Wydane: |
National Academy of Sciences
2020
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| Hasła przedmiotowe: | |
| Dostęp online: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7322008/ https://ncbi.nlm.nih.gov/pubmed/32513703 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1073/pnas.2000317117 |
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