🏠 🔎 © 🔁 ？

MAOAM: Martian Atmosphere Observation and Modeling. v1.104

Data Request

Variable (diurnally averaged)
Time in Ls (from 0° to 360°)
-
Hour at 0 lon. (from 0 h to 23 h)
-
Longitude (from -180° to 180°)
-
Latitude (from -90° to 90°)
-

(from 0 km to 160 km)
-
Scenario
Setting sets
Logarithm format
Value range (only for 2D)
-
Design



The vertical velocities multiplied by 100
Map projection (only for 2D)
Center point (only for sphere)
Lon: Lat:
Colormap (only for 2D)
Get data ⛃

You may be interested in...

Water ice on Mars dependence from Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 210°, Average Lon -180-180°, Summing Height 0-60 km. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Water ice on Mars dependence from Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 210°, Average Lon -180-180°, Summing Height 0-60 km. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Water ice number density on Mars dependence from Latitude -90-90° and Height above
Water ice number density on Mars dependence from Latitude -90-90° and Height above "sea level" 30-90 km in Equirectangular (default) projection with Diurnally averaged, Ls 250°, Average Lon -180-180°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Density on Mars dependence from Time in Ls 0-200° and Height above
Density on Mars dependence from Time in Ls 0-200° and Height above "sea level" 0-150 km in Equirectangular (default) projection with Diurnally averaged, Lon 45°, Lat 0°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Water vapor mix. ratio on Mars dependence from Height above surface 0-160 km in Equirectangular (default) projection with Diurnally averaged, Average Ls 230-270°, Average Lon -180-180°, Lat -80°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Water vapor mix. ratio on Mars dependence from Height above surface 0-160 km in Equirectangular (default) projection with Diurnally averaged, Average Ls 230-270°, Average Lon -180-180°, Lat -80°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Temperature on Mars dependence from Height above surface 0-65 km in Equirectangular (default) projection with Diurnally averaged, Ls 0°, Lon 0°, Lat 0°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Temperature on Mars dependence from Height above surface 0-65 km in Equirectangular (default) projection with Diurnally averaged, Ls 0°, Lon 0°, Lat 0°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Surface temperature on Mars dependence from Latitude 60-90° in Equirectangular (default) projection with Time 0 h, Average Ls 230-312°, Average Lon -180-0°, Height 0 km. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Surface temperature on Mars dependence from Latitude 60-90° in Equirectangular (default) projection with Time 0 h, Average Ls 230-312°, Average Lon -180-0°, Height 0 km. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.