Modeling Jupiter's cloud bands and decks 2. Distribution and motion of condensates
A simple jovian cloud scheme has been developed for the Oxford Planetary Unified model System (OPUS). NH₃-ice, NH₄SH-solid, H₂O-liquid clouds have been modeled in Southern hemisphere limited area simulations of Jupiter. We found that either three or four of the condensates existed in the model. For...
| Главные авторы: | , , |
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| Формат: | Journal article |
| Язык: | English |
| Опубликовано: |
Elsevier
2009
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