🏠 🔎 © 🔁 ？

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...

Water vapor mix. ratio on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 261°, Alt 140 km. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Water vapor mix. ratio on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 261°, Alt 140 km. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Temperature on Mars dependence from Latitude -90-90° and Pressure 0.1-607 Pa in Equirectangular (default) projection with Diurnally averaged, Ls 220°, Lon -90°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Temperature on Mars dependence from Latitude -90-90° and Pressure 0.1-607 Pa in Equirectangular (default) projection with Diurnally averaged, Ls 220°, Lon -90°. 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 170°, 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 170°, Pre 607 Pa. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Temperature on Mars dependence from Latitude -90-90° and Height above surface 0-100 km in Equirectangular (default) projection with Diurnally averaged, Ls 204°, Lon 70°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Temperature on Mars dependence from Latitude -90-90° and Height above surface 0-100 km in Equirectangular (default) projection with Diurnally averaged, Ls 204°, Lon 70°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Water vapor on Mars dependence from Latitude 0-90° and Height above surface 0-100 km in Equirectangular (default) projection with Diurnally averaged, Ls 140°, Average Lon -180-180°. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Water vapor on Mars dependence from Latitude 0-90° and Height above surface 0-100 km in Equirectangular (default) projection with Diurnally averaged, Ls 140°, Average Lon -180-180°. 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 Longitude -180-180° in Equirectangular (default) projection with Diurnally averaged, Lat 60°, Height 0 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°, Height 0 km. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.