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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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Hour at 0 lon. (from 0 h to 23 h)
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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 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 85-95°, 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 85-95°, Average Lon -180-180°. In version 1.074: Water cycle, CO2 cycle, dust bimodal distribution and GW.
Temperature on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Ls 230°, Time (at 0 lon.) 12 h, Height 0 km. In version 1.110: Martian year 28 dust storm (Ls 230 - 312).
Temperature on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Ls 230°, Time (at 0 lon.) 12 h, Height 0 km. In version 1.110: Martian year 28 dust storm (Ls 230 - 312).
Water ice on Mars dependence from Latitude -90-90° and Height above
Water ice on Mars dependence from Latitude -90-90° and Height above "sea level" 0-160 km in Equirectangular (default) projection with Diurnally averaged, Ls 250°, Summing Lon -180-180°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Cell areas on Mars dependence from Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 2°, Lon 0°, Height 0 km. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Cell areas on Mars dependence from Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 2°, Lon 0°, Height 0 km. 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° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 250°, 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° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 250°, Height 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 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 Time in Ls 120-145° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Average Lon -180-180°, Summing Height 0.0000036-607 Pa. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.