Temperature (in K) and wind maps, continued from Figure  1, at pressure levels of 4.4 bar (top) and 20 bar (bottom) in our hot Jupiter model. Maximum wind speeds are 1 (top) and 0.2 km s ⁻¹ (bottom). At these deeper levels, the winds have largely homogenized the longitudinal temperature structure, although some latitudinal gradient remains. The super-rotating equatorial jet descends through much of the atmosphere, down to approximately 7 bar.