MAOAM: Martian Atmosphere Observation and Modeling. v1.029

Data Request

Variable (diurnally averaged)
Time in Ls (from 0° to 360°)
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Longitude (from -180° to 180°)
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Latitude (from -90° to 90°)
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(from 0 km to 160 km)
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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)

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Water vapor mix. ratio on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 235°, Height 60 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 Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 235°, Height 60 km. In version 1.091: Water cycle without molecular diffusion, 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 270°, Lon 26°. 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 270°, Lon 26°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Water ice number density on Mars dependence from Height above surface 1-100 km in Equirectangular (default) projection with Diurnally averaged, Ls 95°, Lon 178°, Lat -21°. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Water ice number density on Mars dependence from Height above surface 1-100 km in Equirectangular (default) projection with Diurnally averaged, Ls 95°, Lon 178°, Lat -21°. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Zonal velocities on Mars dependence from Latitude -90-90° and Height above surface 0-60 km in Equirectangular (default) projection with Diurnally averaged, Ls 40°, 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 Height above surface 0-60 km in Equirectangular (default) projection with Diurnally averaged, Ls 40°, Average Lon -180-180°. In version 1.029: Extended height and CO2 cycle with weak solar acivity.
Water ice on Mars dependence from Time in Ls 0-360° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Average Lon -180-180°, Height 100 km. In version 1.089: Water cycle WITH molecular diffusion, CO2 cycle, dust bimodal distribution and GW.
Water ice on Mars dependence from Time in Ls 0-360° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Average Lon -180-180°, Height 100 km. In version 1.089: Water cycle WITH molecular diffusion, CO2 cycle, dust bimodal distribution and GW.
Surface Water ice on Mars dependence from Longitude -180-180° and Latitude -90-90° in Spherical stereographic projection with Diurnally averaged, Ls 120°, Height 607 Pa. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Surface Water ice on Mars dependence from Longitude -180-180° and Latitude -90-90° in Spherical stereographic projection with Diurnally averaged, Ls 120°, Height 607 Pa. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.