| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10701429 | Icarus | 2012 | 7 Pages |
Abstract
⺠The convective boundary layer (CBL) of Mars is simulated with a 1-D model. ⺠The model results compare well with the Spirit mini-TES temperature profiles. ⺠The sensible and latent heat fluxes H, LE indicate entrainment in the morning hours. ⺠The curving shape of H in the lower CBL can be obtained as a residual.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Hannu Savijärvi,