All experiments simulate an ITCZ at the equator coinciding with the ascending branch of the Hadley circulation, and descending branches at 15°N/S with subtropical jets and easterly trade wind belts straddling the ITCZ. With explicit deep convection, however, rainfall in the ITCZ increases and the Hadley circulation becomes stronger. Increasing horizontal resolution broadens the ITCZ and reduces the differences due to convective treatment. Our diagnostic framework reveals that boundary-layer quasi-equilibrium (BLQE) is a key to physically understanding those differences. At 13km grid spacing, enhanced surface enthalpy fluxes with explicit deep convection are balanced by increased convective downdrafts. As precipitation efficiency is hardly affected, convective updrafts and rainfall increase. The surface enthalpy fluxes are mainly controlled by mean surface winds, closely linked to the Hadley circulation. These links also help understand rainfall differences between different resolutions. At 5km grid spacing, the wind-surface fluxes-convection relation holds, but additionally explicit convection dries the mid-troposphere, which increases the import of air with lower moist static energy into the boundary layer, thereby enhancing surface fluxes. Overall, the different model configurations create little variations in precipitation efficiency and radiative cooling, the effects of which are compensated by changes in dry stability. The results highlight the utility of our diagnostic to pinpoint processes important for rainfall differences between models, suggesting applicability for climate model intercomparison projects.
In addition, we will present results on the behavior of equatorial wave modes in the different aquachannel simulations using time-space filtering and spatial projection methods. Preliminary results show that Kelvin waves are dominant in all simulations, but the simulation modifications change wave characteristics such as wavenumber and propagation speed. Furthermore, one simulation produces an eastward-propagating feature, similar to the Madden-Julian Oscillation.

