| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1775683 | Icarus | 2006 | 5 Pages |
Abstract
The winds of Mars at the water cloud level are measured by tracking cloud features in sequential high-resolution Hubble Space Telescope UV images for 5 days during the perihelion season in 2003. Global circulation model (GCM) predictions are in general agreement with the observations for the zonal wind component, but reveal significant differences for the meridional component.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
V.G. Kaydash, M.A. Kreslavsky, Yu.G. Shkuratov, G. Videen, J.F. III, M. Wolff,