Simulation of temperature maps of Titan at different seasons

These panels are the result of a simulation run with a Global Circulation Model and based on data gathered by Huygens. They show a vertical cross-section of temperatures in the meridional lower atmosphere (at different altitudes) of Titan, during day time. ‘Ls’ (on the image) is the solar longitude describing the season. The temperatures are expressed in Kelvin (0 K= - 273.15 °C)