🏠 🔎 © 🔁 ？

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 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 Time in Ls 0-360° and Latitude 0-10° in Equirectangular (default) projection with Diurnally averaged, Average Lon -180-180°, Alt 0 km. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Water ice on Mars dependence from Time in Ls 0-360° and Latitude 0-10° in Equirectangular (default) projection with Diurnally averaged, Average Lon -180-180°, Alt 0 km. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Water vapor on 6 mbar on Mars dependence from Longitude -180-180° and Height above surface 0-160 km in Equirectangular (default) projection with Diurnally averaged, Average Ls 90-120°, Lat 65°. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Water vapor on 6 mbar on Mars dependence from Longitude -180-180° and Height above surface 0-160 km in Equirectangular (default) projection with Diurnally averaged, Average Ls 90-120°, Lat 65°. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Water vapor mix. ratio on Mars dependence from Time in Ls 0-360° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Lon 0°, Alt 50 km. In version 1.091: Water cycle without molecular diffusion, CO2 cycle, dust bimodal distribution and GW.
Water vapor mix. ratio on Mars dependence from Time in Ls 0-360° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Lon 0°, Alt 50 km. In version 1.091: Water cycle without molecular diffusion, CO2 cycle, dust bimodal distribution and GW.
Absolute horizontal velocities on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Average Ls 0-360°, Height 1 km. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Absolute horizontal velocities on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Average Ls 0-360°, Height 1 km. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Density on Mars dependence from Height above surface 100-160 km in Equirectangular (default) projection with Diurnally averaged, Ls 120°, Lon 0°, Lat 0°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Density on Mars dependence from Height above surface 100-160 km in Equirectangular (default) projection with Diurnally averaged, Ls 120°, 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 Time in Ls 0-360° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Average Lon -180-180°, Pre 50 Pa. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Temperature on Mars dependence from Time in Ls 0-360° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Average Lon -180-180°, Pre 50 Pa. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.