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Dusty Deep Convection in the Mars Year 34 Planet-Encircling Dust Event
Dusty convection, convective activity powered by radiative heating of dust, is a ubiquitous phenomenon in Mars’s atmosphere but is especially deep (that is, impactful on the middle atmosphere) and widespread during planet-encircling dust events (PEDE) that occur every few Mars Years (MY). Yet the re...
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| Publicado no: | J Geophys Res Planets |
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| Main Authors: | , , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
2019
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| Assuntos: | |
| Acesso em linha: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7477802/ https://ncbi.nlm.nih.gov/pubmed/32908808 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1029/2019je006110 |
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