| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1773682 | Icarus | 2012 | 9 Pages |
Abstract
⺠Water vapor abundance at the cloud tops of Venus with high spatial resolution. ⺠At low latitudes mean water vapor abundance is stable and equal to 3 ± 1 ppm. ⺠Scatter and maximum at high latitudes may be explained by dynamic processes. ⺠Water amount contained in a gas phase always dominates that in cloud droplets. ⺠UV markings do not correlate with the cloud tops and water vapor.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
V. Cottini, N.I. Ignatiev, G. Piccioni, P. Drossart, D. Grassi, W.J. Markiewicz,