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)

You may be interested in...

Water ice on Mars dependence from Time in Ls 120-145° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Average Lon -180-180°, Summing Alt 0.0000036-607 Pa. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Water ice on Mars dependence from Time in Ls 120-145° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Average Lon -180-180°, Summing Alt 0.0000036-607 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 0°, Summing Height 0-40 km. 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 0°, Summing Height 0-40 km. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Dust number density (given) on Mars dependence from Longitude -180-180° in Equirectangular (default) projection with Diurnally averaged, Ls 250°, Lat -30°, Height 607 Pa. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Dust number density (given) on Mars dependence from Longitude -180-180° in Equirectangular (default) projection with Diurnally averaged, Ls 250°, Lat -30°, Height 607 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°, Alt 100 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 Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Average Lon -180-180°, Alt 100 km. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Zonal velocities on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 306°, Height 100 km. In version 1.091: Water cycle without molecular diffusion, CO2 cycle, dust bimodal distribution and GW.
Zonal velocities on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 306°, Height 100 km. In version 1.091: Water cycle without molecular diffusion, CO2 cycle, dust bimodal distribution and GW.
Dust number density (given) on Mars dependence from Time in Ls 0-10° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Average Lon -180-180°, Height 10 km. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Dust number density (given) on Mars dependence from Time in Ls 0-10° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Average Lon -180-180°, Height 10 km. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.