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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 km to 160 km)
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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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Water ice on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 120°, Height 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 120°, Height 607 Pa. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Water ice mix. ratio on Mars dependence from Longitude -180-180° and Latitude 50-90° in North polar stereographic projection with Diurnally averaged, Average Ls 90-120°, Average Height 0.0000036-607 Pa. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Water ice mix. ratio on Mars dependence from Longitude -180-180° and Latitude 50-90° in North polar stereographic projection with Diurnally averaged, Average Ls 90-120°, Average Height 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 Latitude -90-90° and Hybrid model levels 10-607 Pa in Equirectangular (default) projection with Diurnally averaged, Ls 130°, Average Lon -180-180°. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Water ice on Mars dependence from Latitude -90-90° and Hybrid model levels 10-607 Pa in Equirectangular (default) projection with Diurnally averaged, Ls 130°, Average Lon -180-180°. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Water vapor mix. ratio on Mars dependence from Longitude -180-180° and Latitude -10-90° in North polar stereographic projection with Diurnally averaged, Ls 76°, Alt 10 km. In version 1.089: Water cycle WITH molecular diffusion, CO2 cycle, dust bimodal distribution and GW.
Water vapor mix. ratio on Mars dependence from Longitude -180-180° and Latitude -10-90° in North polar stereographic projection with Diurnally averaged, Ls 76°, Alt 10 km. In version 1.089: Water cycle WITH molecular diffusion, CO2 cycle, dust bimodal distribution and GW.
Dust opacity (given) on Mars dependence from Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 270°, Lon 70°, Height 0 km. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Dust opacity (given) on Mars dependence from Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 270°, Lon 70°, Height 0 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 Time in Ls 0-360° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Average Lon -180-180°, Alt 120 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, Average Lon -180-180°, Alt 120 km. In version 1.091: Water cycle without molecular diffusion, CO2 cycle, dust bimodal distribution and GW.