Rate of change of temperature or heating profiles, known as temperature increments, plotted against σ (pressure divided by surface pressure) for simulations T1:T1e (solid lines), ProC:T1e (dashed lines), and Sun:T1e (dotted lines) for each component process. The processes shown are atmospheric absorption of stellar radiation (orange, top panels),thermal emission or absorption of planetary radiation (grey, top panels), large-scale circulation, known as advection, (pink, bottom panels), latent heating or cooling of water (blue, bottom panels), and turbulent mixing (green, bottom panels). The day- and nightside hemispherically averaged values are shown in the left and right panels, respectively.The x-axis limits are different between the day- and nightside panels. In equilibrium the net heating is zero.