MAOAM: Martian Atmosphere Observation and Modeling. v1.104
You may be interested in...
Absolute horizontal velocities on Mars dependence from Latitude -90-90° and Height above surface 0-5 km in Equirectangular (default) projection with Diurnally averaged, Average Ls 0-360°, Lon 0°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Zonal velocities on Mars dependence from Latitude -50-85° and Pressure 0.1-607 Pa in Equirectangular (default) projection with Diurnally averaged, Ls 230°, Lon -120°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Water ice on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 130°, Pre 607 Pa. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Absolute horizontal velocities on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 170°, Pre 607 Pa. In version 1.089: Water cycle WITH molecular diffusion, CO2 cycle, dust bimodal distribution and GW.
Temperature on Mars dependence from Height above surface 0-160 km in Equirectangular (default) projection with Diurnally averaged, Ls 120°, Lon 90°, Lat 90°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Water vapor mix. ratio on Mars dependence from Latitude -90-90° and Height above surface 5-50 km in Equirectangular (default) projection with Diurnally averaged, Average Ls 45-60°, Average Lon -180-180°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.