Abstract
Venus global-scale H2SO4 cloud and haze layers form via the combination of SO3 and H2O, and SO3 forms via oxidation of SO2. Sulfurbearing and sulfur-oxidized species, such as SO2, SO, S, OCS, H2SO4, are key traces of Venus H2SO4 cloud/haze formation process.
| Original language | English |
|---|---|
| Pages (from-to) | 2pp |
| Journal | 47th Lunar and Planetary Science Conference |
| DOIs | |
| Publication status | Published - 2016 |
| Event | 47th Lunar and Planetary Science Conference - The Woodlands, Texas, USA Duration: 1 Jan 2016 → … |