Physical mechanisms controlling self-aggregation of convection in idealized numerical modeling simulations

We elucidate the physics of self-aggregation by applying a new diagnostic technique to the output of a cloud resolving model. Specifically, the System for Atmospheric Modeling is used to perform 3-d cloud system resolving simulations of radiative-convective equilibrium in a non-rotating framework, with interactive radiation and surface fluxes and fixed sea surface temperature (SST). We introduce a novel method to quantify the magnitudes of the various feedbacks that control self-aggregation within the framework of the budget for the spatial variance of column - integrated frozen moist static energy. The absorption of shortwave radiation by atmospheric water vapor is found to be a key positive feedback in the evolution of aggregation. In addition, we find a positive wind speed-surface flux feedback whose role is to counteract a negative feedback due to the effect of air-sea enthalpy disequilibrium on surface fluxes. The longwave radiation feedback can be either positive or negative in the early stages of aggregation; however, it is the dominant positive feedback that maintains the aggregated state once it develops. Importantly, we find that the mechanisms that maintain the aggregate state are distinct from those that instigate the evolution of self-aggregation. Finally, we note that self-aggregation begins as a dry patch that expands, eventually forcing all the convection into a single clump. Thus, we focus on processes that can amplify this initial dry patch.