One-dimensional Microphysics Model of Venusian Clouds from 40 to 100 km: Impact of the Middle-atmosphere Eddy Transport and SOIR Temperature Profile on the Cloud Structure
We conducted a simulation of H _2 SO _4 vapor, H _2 O vapor, and H _2 SO _4 –H _2 O liquid aerosols from 40 to 100 km, using a 1D Venus cloud microphysics model based on the one detailed in Imamura & Hashimoto. The cloud distribution obtained is in good agreement with in situ observations by Pioneer...
Kaydedildi:
| Asıl Yazarlar: | , , , , , , |
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| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
IOP Publishing
2024-01-01
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| Seri Bilgileri: | The Planetary Science Journal |
| Konular: | |
| Online Erişim: | https://doi.org/10.3847/PSJ/ad25f3 |
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