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MAOAM: Martian Atmosphere Observation and Modeling. v1.104

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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Surface temperature on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Time 0 h, Ls 270°, Alt 0 km. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Surface temperature on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Time 0 h, Ls 270°, Alt 0 km. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Water ice on Mars dependence from Latitude -90-90° and Pressure 0.0000036-607 Pa in Equirectangular (default) projection with Diurnally averaged, Ls 270°, Average Lon -180-180°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Water ice on Mars dependence from Latitude -90-90° and Pressure 0.0000036-607 Pa in Equirectangular (default) projection with Diurnally averaged, Ls 270°, Average Lon -180-180°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Meridional velocities on Mars dependence from Latitude -90-90° and Height above surface 30-160 km in Equirectangular (default) projection with Diurnally averaged, Ls 300°, Average Lon -180-180°. In version 1.074: Water cycle, CO2 cycle, dust bimodal distribution and GW.
Meridional velocities on Mars dependence from Latitude -90-90° and Height above surface 30-160 km in Equirectangular (default) projection with Diurnally averaged, Ls 300°, Average Lon -180-180°. In version 1.074: Water cycle, CO2 cycle, dust bimodal distribution and GW.
Surface Water ice on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 100°, Height 0 km. 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 Equirectangular (default) projection with Diurnally averaged, Ls 100°, Height 0 km. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Surface Water ice on Mars dependence from Time in Ls 0-360° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Lon 0°, Height 0 km. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Surface Water ice on Mars dependence from Time in Ls 0-360° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Lon 0°, Height 0 km. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Density on Mars dependence from Latitude -90-90° and Height above
Density on Mars dependence from Latitude -90-90° and Height above "sea level" 0-150 km in Equirectangular (default) projection with Diurnally averaged, Ls 0°, Lon -60°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.