Загрузка...
The puzzling Venusian polar atmospheric structure reproduced by a general circulation model
Unlike the polar vortices observed in the Earth, Mars and Titan atmospheres, the observed Venus polar vortex is warmer than the midlatitudes at cloud-top levels (∼65 km). This warm polar vortex is zonally surrounded by a cold latitude band located at ∼60° latitude, which is a unique feature called ‘...
Сохранить в:
| Опубликовано в: : | Nat Commun |
|---|---|
| Главные авторы: | , , , , , |
| Формат: | Artigo |
| Язык: | Inglês |
| Опубликовано: |
Nature Publishing Group
2016
|
| Предметы: | |
| Online-ссылка: | https://ncbi.nlm.nih.gov/pmc/articles/PMC4740379/ https://ncbi.nlm.nih.gov/pubmed/26832195 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1038/ncomms10398 |
| Метки: |
Добавить метку
Нет меток, Требуется 1-ая метка записи!
|