| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 5488070 | Planetary and Space Science | 2016 | 18 Pages |
Abstract
Our new radiative scheme is more suitable for 3D Venus climate models than those used in previous work due to its easy adaptability to different atmospheric conditions. This flexibility of the model was crucial to explore the uncertainties in the lower atmospheric conditions and may also be used in the future to explore, for example, dynamical-radiative-microphysical feedbacks.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
J.M. Mendonça, P.L. Read,