🏠 🔎 © 🔁 ？

MAOAM: Martian Atmosphere Observation and Modeling. v1.058

Data Request

Variable (diurnally averaged)
Time in Ls (from 0° to 360°)
-
Longitude (from -180° to 180°)
-
Latitude (from -90° to 90°)
-
(from 0.0000036 Pa to 607 Pa)
-
Scenario
Setting sets
Logarithm format
Value range (only for 2D)
-
Design



The vertical velocities multiplied by 100
Map projection (only for 2D)
Center point (only for sphere)
Lon: Lat:
Colormap (only for 2D)
Get data ⛃

You may be interested in...

Surface pressure on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 1°, Lev 607 Pa. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Surface pressure on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 1°, Lev 607 Pa. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Zonal velocities on Mars dependence from Latitude -90-90° and Height above surface 0-160 km in Equirectangular (default) projection with Diurnally averaged, Ls 68°, Average Lon -180-180°. In version 1.029: Extended height and CO2 cycle with weak solar acivity.
Zonal velocities on Mars dependence from Latitude -90-90° and Height above surface 0-160 km in Equirectangular (default) projection with Diurnally averaged, Ls 68°, Average Lon -180-180°. In version 1.029: Extended height and CO2 cycle with weak solar acivity.
Water vapor on Mars dependence from Longitude -180-180° and Latitude 0-90° in North polar stereographic projection with Diurnally averaged, Ls 170°, Summing Height 3-120 km. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Water vapor on Mars dependence from Longitude -180-180° and Latitude 0-90° in North polar stereographic projection with Diurnally averaged, Ls 170°, Summing Height 3-120 km. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Water ice number density on Mars dependence from Time in Ls 0-10° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Average Lon -180-180°, Height 10 km. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Water ice number density on Mars dependence from Time in Ls 0-10° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Average Lon -180-180°, Height 10 km. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Water vapor on Mars dependence from Time in Ls 0-360° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Average Lon -180-180°, Height 160 km. In version 1.058: Limited height with water cycle, weak diffusion and dust bimodal distribution.
Water vapor on Mars dependence from Time in Ls 0-360° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Average Lon -180-180°, Height 160 km. 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 0.0001-607 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 0.0001-607 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.