🏠 🔎 © 🔁 ？

MAOAM: Martian Atmosphere Observation and Modeling. v1.058

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 0.0000036 Pa to 607 Pa)
-
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...

Temperature on Mars dependence from Time in Ls 0-360° and Longitude -180-180° in Equirectangular (default) projection with Diurnally averaged, Lat -60°, Alt 130 km. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Temperature on Mars dependence from Time in Ls 0-360° and Longitude -180-180° in Equirectangular (default) projection with Diurnally averaged, Lat -60°, Alt 130 km. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Surface pressure on Mars dependence from Longitude -180-180° and Latitude -80-80° in Equirectangular (default) projection with Diurnally averaged, Average Ls 0-360°, Pre 607 Pa. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Surface pressure on Mars dependence from Longitude -180-180° and Latitude -80-80° in Equirectangular (default) projection with Diurnally averaged, Average Ls 0-360°, Pre 607 Pa. 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.
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.
Temperature on Mars dependence from Longitude -180-180° and Height above surface 0-150 km in Equirectangular (default) projection with Diurnally averaged, Ls 0°, Lat 45°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Temperature on Mars dependence from Longitude -180-180° and Height above surface 0-150 km in Equirectangular (default) projection with Diurnally averaged, Ls 0°, Lat 45°. 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 -23-23° and Height above surface 0-10 km in Equirectangular (default) projection with Diurnally averaged, Ls 22.9°, Lon 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 Latitude -23-23° and Height above surface 0-10 km in Equirectangular (default) projection with Diurnally averaged, Ls 22.9°, Lon 0°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Vertical velocities on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 266°, Height 60 km. In version 1.091: Water cycle without molecular diffusion, CO2 cycle, dust bimodal distribution and GW.
Vertical velocities on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 266°, Height 60 km. In version 1.091: Water cycle without molecular diffusion, CO2 cycle, dust bimodal distribution and GW.