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Numerical experiments are conducted using the University of Illinois, Urbana–Champaign (UIUC), 11-layer atmospheric general circulation model (GCM) to investigate the dependence of the simulated tropical intraseasonal oscillation (TIO) on convection parameterization. Three convection parameterizations have been tested: 1) the UIUC GCM's original cumulus–convection parameterization, which includes a modified version of the penetrative–convection parameterization and a middle-level convection parameterization, 2) the parameterization of , and (3) the moist convective adjustment parameterization of For each parameterization a relative humidity criterion (RHc) for convection or convective heating to occur is used, as in many GCMs. Perpetual-March simulations with these convection parameterizations have been performed for different values of RHc. It is found that the simulated TIO is highly dependent on RHc. As RHc increases, the oscillation in the simulations becomes stronger for all three parameterizations. This dependence of the amplitude of the simulated oscillation on RHc appears to explain the differences in the TIO among previous simulations by different GCMs. The analysis of the simulations suggests that a certain degree of nonlinear dependence of the condensational heating on large-scale moisture convergence is required to give a reasonable simulation of the TIO. When large values of RHc are used, the triggering of convective activity requires the moist static energy in the lower troposphere to be accumulated to a certain amount through moisture convergence. This requirement of accumulation of the moist static energy to trigger convection leads to the weakening of the interaction between the circulation and the heating for perturbations of small amplitudes and small scales, and allows the initiation of the TIO to occur at lower frequencies. In the simulations that produce relatively strong intraseasonal oscillations, the frictional wave-CISK (conditional instability of the second kind) appears to contribute to the amplification of the TIO.
Wang et al. (Sat,) studied this question.