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MAOAM: Martian Atmosphere Observation and Modeling. v1.058

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 0.0000036 Pa to 607 Pa)
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Scenario
Setting sets
Logarithm format
Value range (only for 2D)
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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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Temperature on Mars dependence from Latitude -90-90° and Height above surface 0-100 km in Equirectangular (default) projection with Diurnally averaged, Ls 100°, Lon 0°. 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 100°, Lon 0°. In version 1.091: Water cycle without molecular diffusion, CO2 cycle, dust bimodal distribution and GW.
Cell heights on Mars dependence from Latitude -90-90° and Height above surface 0-160 km in Equirectangular (default) projection with Diurnally averaged, Ls 120°, Lon 90°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Cell heights on Mars dependence from Latitude -90-90° and Height above surface 0-160 km in Equirectangular (default) projection with Diurnally averaged, Ls 120°, Lon 90°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Water ice number density on Mars dependence from Time in Ls 0-360° and Height above surface 0-160 km in Equirectangular (default) projection with Diurnally averaged, Lon 0°, Lat -50°. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Water ice number density on Mars dependence from Time in Ls 0-360° and Height above surface 0-160 km in Equirectangular (default) projection with Diurnally averaged, Lon 0°, Lat -50°. 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 -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 140°, Summing Height 10-160 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 -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 140°, Summing Height 10-160 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 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.
Temperature on Mars dependence from Latitude -90-90° and Height above surface 0-160 km in Equirectangular (default) projection with Diurnally averaged, Ls 120°, Lon 100°. 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 0-160 km in Equirectangular (default) projection with Diurnally averaged, Ls 120°, Lon 100°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.