| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1773976 | Icarus | 2011 | 7 Pages |
Abstract
⺠Vertical profiles of H2SO4 concentration and densities of H2SO4 vapor at 70-110 km on Venus. ⺠H2SO4 vapor cannot be a high-altitude source of SOX on Venus. ⺠Haze extinction may contaminate the UV observations of SO2 at 90-110 km.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Vladimir A. Krasnopolsky,
