Author/Authors :
Kaydash، نويسنده , , V.G. and Kreslavsky، نويسنده , , M.A. and Shkuratov، نويسنده , , Yu.G. and Videen، نويسنده , , G. and Bell III، نويسنده , , J.F and Wolff، نويسنده , , M.، نويسنده ,
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.
