These panels are the result of a simulation run with a Global Circulation Model and based on data gathered by Huygens. The panels provide an instantaneous global map of temperature (first three rows) and surface pressure (last row) for the time of the probe’s descent onto Titan.
The temperature maps were simulated for different altitudes: 4.5 kilometres, 300 metres, and ground, respectively. The pressure is simulated for the ground level.
The left column shows the results taking into account Saturn’s tidal force, the right column the results without Saturn’s tide