| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1773683 | Icarus | 2012 | 15 Pages |
Abstract
⺠We present 2D-spatial maps of venusian CO distribution. ⺠A general trend of increased CO abundances at 60° latitude is found, in line with previous reports. ⺠Significant changes are seen in distribution maps over long periods. ⺠The spectrum is modeled to reveal the altitude of CO variation. ⺠Excess CO occurs at around 45 km, not 35 km as previously assumed.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Daniel V. Cotton, Jeremy Bailey, D. Crisp, V.S. Meadows,