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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 0.0000036 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 10-50 km in Equirectangular (default) projection with Ls 280°, Time (at 0 lon.) 15 h, Lon 1°. In version 1.110: Martian year 28 dust storm (Ls 230 - 312).
Temperature on Mars dependence from Latitude -90-90° and Height above surface 10-50 km in Equirectangular (default) projection with Ls 280°, Time (at 0 lon.) 15 h, Lon 1°. In version 1.110: Martian year 28 dust storm (Ls 230 - 312).
Zonal velocities on Mars dependence from Longitude -127--87° and Latitude -13-7° in Equirectangular (default) projection with Diurnally averaged, Ls 170°, Height 607 Pa. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Zonal velocities on Mars dependence from Longitude -127--87° and Latitude -13-7° in Equirectangular (default) projection with Diurnally averaged, Ls 170°, Height 607 Pa. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Zonal velocities on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 266°, Height 90 km. In version 1.091: Water cycle without molecular diffusion, CO2 cycle, dust bimodal distribution and GW.
Zonal velocities on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 266°, Height 90 km. In version 1.091: Water cycle without molecular diffusion, CO2 cycle, dust bimodal distribution and GW.
Density on Mars dependence from Height above
Density on Mars dependence from Height above "sea level" 0-150 km in Equirectangular (default) projection with Diurnally averaged, Ls 90°, Lon 0°, Lat 45°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Absolute horizontal velocities on Mars dependence from Latitude -90--30° and Height above
Absolute horizontal velocities on Mars dependence from Latitude -90--30° and Height above "sea level" 0-160 km in Equirectangular (default) projection with Diurnally averaged, Ls 260°, Average Lon -180-180°. In version 1.089: Water cycle WITH molecular diffusion, CO2 cycle, dust bimodal distribution and GW.
Vertical velocities on Mars dependence from Latitude -90-90° and Height above
Vertical velocities on Mars dependence from Latitude -90-90° and Height above "sea level" 0-160 km in Equirectangular (default) projection with Diurnally averaged, Ls 40°, Average Lon -180-180°. In version 1.029: Extended height and CO2 cycle with weak solar acivity.