3. Results

The dependency of the structure of the three-dimensional gray atmosphere on the solar constant and the runaway greenhouse states. 3.c. Changes in the Equilibrium State (Circulation Pattern) 3.e. Changes in the Equilibrium State (Precipitation Distribution)

d. Changes in the Equilibrium State (Meridional Structure)

As a preparatory step in identifying what determines the runaway limit, the meridional structures of OLR and surface temperature in the equilibrium state with increasing the value of solar constant will be summarized. Figure 1 shows the meridional distribution of the zonal mean OLR and zonal mean surface temperature for experiments S1200, S1380, S1500, S1550, and S1570. The following observations can be made based on the figure.

Based on the above results, it may be concluded that the meridional contrast in the thermal structure of the atmosphere is reduced with increases in solar constant.

figure 1
Figure 1: The meridional distribution of the zonal mean OLR (W/m2, green line) and zonal mean surface temperature (K, red line) in equilibrium states for experiments S1200, S1380, S1500, S1550, and S1570.


3.d. Changes in the Equilibrium State (Meridional Structure) The dependency of the structure of the three-dimensional gray atmosphere on the solar constant and the runaway greenhouse states. 3.c. Changes in the Equilibrium State (Circulation Pattern) 3.e. Changes in the Equilibrium State (Precipitation Distribution)