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.
Original language | English (US) |
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Pages (from-to) | 97-101 |
Number of pages | 5 |
Journal | Icarus |
Volume | 185 |
Issue number | 1 |
DOIs | |
State | Published - Nov 2006 |
Externally published | Yes |
Keywords
- Atmospheres
- Mars
- Ultraviolet observations
- climate
- dynamics
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science