🏠 🔎 © 🔁 ？

MAOAM: Martian Atmosphere Observation and Modeling. v1.058

Data Request

Variable (diurnally averaged)
Time in Ls (from 0° to 360°)
-
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 vapor on Mars dependence from Longitude -180-180° and Latitude 0-90° in North polar stereographic projection with Diurnally averaged, Ls 100°, Summing Height 0-70 km. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Water vapor on Mars dependence from Longitude -180-180° and Latitude 0-90° in North polar stereographic projection with Diurnally averaged, Ls 100°, Summing Height 0-70 km. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Water vapor on Mars dependence from Time in Ls 0-180° in Equirectangular (default) projection with Diurnally averaged, Average Lon -180-180°, Lat 70°, Summing Height 0-100 km. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Water vapor on Mars dependence from Time in Ls 0-180° in Equirectangular (default) projection with Diurnally averaged, Average Lon -180-180°, Lat 70°, Summing Height 0-100 km. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Surface CO2 ice on Mars dependence from Longitude -180-180° and Latitude -90--50° in South polar stereographic projection with Time 0 h, Ls 150°, Height 0 km. In version 1.089: Water cycle WITH molecular diffusion, CO2 cycle, dust bimodal distribution and GW.
Surface CO2 ice on Mars dependence from Longitude -180-180° and Latitude -90--50° in South polar stereographic projection with Time 0 h, Ls 150°, Height 0 km. In version 1.089: Water cycle WITH molecular diffusion, CO2 cycle, dust bimodal distribution and GW.
Zonal velocities on Mars dependence from Latitude -90-90° and Pressure 0.0000036-607 Pa in Equirectangular (default) projection with Diurnally averaged, Ls 70°, Average Lon -180-180°. In version 1.029: Extended height and CO2 cycle with weak solar acivity.
Zonal velocities on Mars dependence from Latitude -90-90° and Pressure 0.0000036-607 Pa in Equirectangular (default) projection with Diurnally averaged, Ls 70°, Average Lon -180-180°. In version 1.029: Extended height and CO2 cycle with weak solar acivity.
Water vapor mix. ratio on Mars dependence from Latitude -90-90° and Pressure 0.0000036-607 Pa in Equirectangular (default) projection with Diurnally averaged, Average Ls 355-360°, Average Lon -180-180°. In version 1.074: Water cycle, CO2 cycle, dust bimodal distribution and GW.
Water vapor mix. ratio on Mars dependence from Latitude -90-90° and Pressure 0.0000036-607 Pa in Equirectangular (default) projection with Diurnally averaged, Average Ls 355-360°, Average Lon -180-180°. In version 1.074: Water cycle, 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.
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.