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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Surface CO2 ice on Mars dependence from Longitude -180-180° and Latitude -90--70° in South polar stereographic projection with Time 0 h, Ls 100°, Height 0 km. In version 1.089: Water cycle WITH molecular diffusion, CO2 cycle, dust bimodal distribution and GW.
Surface CO2 ice on Mars dependence from Longitude -180-180° and Latitude -90--70° in South polar stereographic projection with Time 0 h, Ls 100°, Height 0 km. In version 1.089: Water cycle WITH molecular diffusion, CO2 cycle, dust bimodal distribution and GW.
Water ice number density on Mars dependence from Height above surface 0-100 km in Equirectangular (default) projection with Diurnally averaged, Average Ls 0-360°, Lon 0°, Lat 0°. 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 0-100 km in Equirectangular (default) projection with Diurnally averaged, Average Ls 0-360°, Lon 0°, Lat 0°. 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 Height above surface 0-160 km in Equirectangular (default) projection with Diurnally averaged, Ls 270°, Lon 90°. 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 Height above surface 0-160 km in Equirectangular (default) projection with Diurnally averaged, Ls 270°, Lon 90°. 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 Average Ls 240-243°, Time (at 0 lon.) 0 h, Height 0 km. In version 1.110: Martian year 28 dust storm (Ls 230 - 312).
Surface temperature on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Average Ls 240-243°, Time (at 0 lon.) 0 h, Height 0 km. In version 1.110: Martian year 28 dust storm (Ls 230 - 312).
Temperature on Mars dependence from Hour at 0 lon. 0-23 h and Height above surface 0-1 km in Equirectangular (default) projection with Ls 185°, Lon 137.4°, Lat -4.6°. In version 1.114: Martian year 34 dust storm (Ls 185 - 267).
Temperature on Mars dependence from Hour at 0 lon. 0-23 h and Height above surface 0-1 km in Equirectangular (default) projection with Ls 185°, Lon 137.4°, Lat -4.6°. In version 1.114: Martian year 34 dust storm (Ls 185 - 267).
Temperature on Mars dependence from Height above surface 0-1 km in Equirectangular (default) projection with Ls 270°, Time (at 0 lon.) 6 h, Lon 0°, Lat 0°. In version 1.110: Martian year 28 dust storm (Ls 230 - 312).
Temperature on Mars dependence from Height above surface 0-1 km in Equirectangular (default) projection with Ls 270°, Time (at 0 lon.) 6 h, Lon 0°, Lat 0°. In version 1.110: Martian year 28 dust storm (Ls 230 - 312).