Abstract

We have developed a spectral cumulus parameterization using a cloud-resolving model. This includes a new parameterization of the entrainment rate which was derived from analysis of the cloud properties obtained from the cloud-resolving model simulation and was valid for both shallow and deep convection. The new scheme was examined in a single-column model experiment and compared with the existing parameterization of Gregory (2001, Q J R Meteorol Soc 127:53–72) (GR scheme). The results showed that the GR scheme simulated more shallow and diluted convection than the new scheme. To further validate the physical performance of the parameterizations, Atmospheric Model Intercomparison Project (AMIP) experiments were performed, and the results were compared with reanalysis data. The new scheme performed better than the GR scheme in terms of mean state and variability of atmospheric circulation, i.e., the new scheme improved positive bias of precipitation in western Pacific region, and improved positive bias of outgoing shortwave radiation over the ocean. The new scheme also simulated better features of convectively coupled equatorial waves and Madden–Julian oscillation. These improvements were found to be derived from the modification of parameterization for the entrainment rate, i.e., the proposed parameterization suppressed excessive increase of entrainment, thus suppressing excessive increase of low-level clouds.

Highlights

  • The cumulus parameterization is responsible for reproducing tropical convection, and convectively coupled equatorial waves (CCEWs) and Madden–Julian oscillation (MJO; Madden and Julian 1971) which play important roles in global atmospheric circulation

  • The new scheme simulated larger convective available potential energy (CAPE) than the GR scheme, and much deeper clouds are more significant than the GR scheme

  • The new scheme simulated larger convective heating and drying rates up to 400 mb level. This indicates that deeper convective clouds are more significant in the new scheme than that in the GR scheme

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Summary

Introduction

The cumulus parameterization is responsible for reproducing tropical convection, and convectively coupled equatorial waves (CCEWs) and Madden–Julian oscillation (MJO; Madden and Julian 1971) which play important roles in global atmospheric circulation. Simulations of these phenomena are still considered difficult for even recent general circulation models (GCMs), since they involve a lot of unresolved cloud-related processes and still contain many uncertainties (e.g., Kim et al 2009; Weaver et al 2011). Deep and shallow convection can coexist, and the parameterization should be able to express different cloud types and their coexistence. The best approach to expressing this coexistence has not yet been determined

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