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Convective storms and atmospheric vertical structure in Uranus and Neptune
The ice giants Uranus and Neptune have hydrogen-based atmospheres with several constituents that condense in their cold upper atmospheres. A small number of bright cloud systems observed in both planets are good candidates for moist convective storms, but their observed properties (size, temporal sc...
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| Publicado en: | Philos Trans A Math Phys Eng Sci |
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| Autores principales: | , , |
| Formato: | Artigo |
| Lenguaje: | Inglês |
| Publicado: |
The Royal Society Publishing
2020
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| Materias: | |
| Acceso en línea: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7658788/ https://ncbi.nlm.nih.gov/pubmed/33161859 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1098/rsta.2019.0476 |
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