Meteorological variability and the annual surface pressure cycle on Mars

It is commonly admitted that the seasonal surface pressure cycle, observed on Mars by the two Viking landers, is due to condensation and sublimation of the atmospheric carbon dioxide in the polar caps. A three Martian year numerical simulation has been performed with a Martian General Circulation Model. The results, validated by comparison to Viking pressure measurements and to temperature fields retrieved from Mariner-9 measurements, show that the pressure cycle depends on the location of the planet. They strongly suggest that, in addition to condensation and sublimation of the atmospheric carbon dixoide, two other effects significantly contribute to the pressure cycle: an orographic effect resulting from the difference in mean height between the two hemispheres, and a dynamical effect resulting from the geographic balance between the mass and wind field. -from Authors