🏠 🔎 © 🔁 ？

MAOAM: Martian Atmosphere Observation and Modeling. v1.058

Data Request

Variable (diurnally averaged)
Time in Ls (from 0° to 360°)
-
Hour at 0 lon. (from 0 h to 23 h)
-
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...

Pressure on Mars dependence from Latitude -90-90° and Height above surface 0-160 km in Equirectangular (default) projection with Diurnally averaged, Ls 270°, Average Lon 0-180°. In version 1.029: Extended height and CO2 cycle with weak solar acivity.
Pressure on Mars dependence from Latitude -90-90° and Height above surface 0-160 km in Equirectangular (default) projection with Diurnally averaged, Ls 270°, Average Lon 0-180°. In version 1.029: Extended height and CO2 cycle with weak solar acivity.
Density on Mars dependence from Longitude -180-180° and Height above surface 0-100 km in Equirectangular (default) projection with Diurnally averaged, Ls 90°, Lat 80°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Density on Mars dependence from Longitude -180-180° and Height above surface 0-100 km in Equirectangular (default) projection with Diurnally averaged, Ls 90°, Lat 80°. 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 250°, 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 Height above surface 0-160 km in Equirectangular (default) projection with Diurnally averaged, Ls 250°, Average Lon -180-180°. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Water vapor mix. ratio on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 125°, Height 30 km. In version 1.091: Water cycle without molecular diffusion, CO2 cycle, dust bimodal distribution and GW.
Water vapor mix. ratio on Mars dependence from Longitude -180-180° and Latitude -90-90° in Equirectangular (default) projection with Diurnally averaged, Ls 125°, Height 30 km. In version 1.091: Water cycle without molecular diffusion, CO2 cycle, dust bimodal distribution and GW.
Temperature on Mars dependence from Longitude 135-155° and Latitude 22-35° in Equirectangular (default) projection with Diurnally averaged, Ls 75°, Height 70 km. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Temperature on Mars dependence from Longitude 135-155° and Latitude 22-35° in Equirectangular (default) projection with Diurnally averaged, Ls 75°, Height 70 km. In version 1.104: Water cycle for annual dust, CO2 cycle, dust bimodal distribution and GW.
Temperature on Mars dependence from Hour at 0 lon. 0-23 h and Height above surface 0-160 km in Equirectangular (default) projection with Ls 267°, Lon 0°, Lat 0°. 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 0-160 km in Equirectangular (default) projection with Ls 267°, Lon 0°, Lat 0°. In version 1.110: Martian year 28 dust storm (Ls 230 - 312).