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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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| 出版年: | Proc Natl Acad Sci U S A |
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| 主要な著者: | , |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
National Academy of Sciences
2020
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| 主題: | |
| オンライン･アクセス: | 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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