| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1773936 | Icarus | 2011 | 14 Pages |
Abstract
⺠The present work shows significances of microscale dynamics in Venus atmospheric modeling. ⺠Venus' near-surface thermal structure is controlled by convective adjustment and mixing. ⺠The convective adjustment and mixing produce large eddy diffusion coefficients in PBL. ⺠The mixed layer may fully develop if surface heat flux is high around volcanic hotspots.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Masaru Yamamoto,