Abstract

The effect of the air–sea interaction on the Madden–Julian Oscillation (MJO) was investigated using the one-column ocean model Snow–Ice–Thermocline (SIT 1.06) embedded in the Community Atmosphere Model 5.3 (CAM5.3; hereafter CAM5–SIT v1.0). The SIT model with 41 vertical layers was developed to simulate sea surface temperature (SST) and upper-ocean temperature variations with a high vertical resolution that resolves the cool skin and diurnal warm layer and the upper oceanic mixed layer. A series of 30-year sensitivity experiments were conducted in which various model configurations (e.g., coupled versus uncoupled, vertical resolution and depth of the SIT model, coupling domains, and absence of the diurnal cycle) were considered to evaluate the effect of air–sea coupling on MJO simulation. Most of the CAM5–SIT experiments exhibited higher fidelity than the CAM5-alone experiment in characterizing the basic features of the MJO such as spatiotemporal variability and the eastward propagation in boreal winter. The overall MJO simulation performance of CAM5–SIT benefited from (1) better resolving the fine structure of upper-ocean temperature and therefore the air–sea interaction that resulted in more realistic intraseasonal variability in both SST and atmospheric circulation and (2) the adequate thickness and vertical resolution of the oceanic mixed layer. The sensitivity experiments demonstrated the necessity of coupling the tropical eastern Pacific in addition to the tropical Indian Ocean and the tropical western Pacific. Enhanced MJO could be obtained without considering the diurnal cycle in coupling.

Highlights

  • The Madden–Julian Oscillation (MJO) is a tropical large-scale convection circulation system that propagates eastward across the warm pool region from the tropical Indian Ocean (IO) to the western Pacific (WP) on an intraseasonal time scale (Madden and Julian, 1972)

  • With that of the uncoupled atmospheric general circulation models (AGCMs) (A–CTL) forced by climatological monthly sea surface temperature (SST) to demonstrate the effect of air–sea coupling on the MJO simulation by coupling the SIT

  • A wavenumber–frequency spectrum (W–FS) analysis was conducted to quantify propagation characteristics simulated in different experiments

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Summary

Introduction

The Madden–Julian Oscillation (MJO) is a tropical large-scale convection circulation system that propagates eastward across the warm pool region from the tropical Indian Ocean (IO) to the western Pacific (WP) on an intraseasonal time scale (Madden and Julian, 1972). During the suppression of convection, the MJO propagates eastward with light winds, which is accompanied by enhanced downwelling shortwave radiation absorption, weaker upward latent and sensible fluxes, less cloudiness and precipitation, and weaker vertical mixing in the upper ocean, causing an increase in the upper-ocean temperature. In the following active phase when deep convection occurs, downwelling shortwave radiation is reduced and stronger westerly winds enhance evaporation and sensible heat loss from the ocean surface, causing a decrease in the upper-ocean temperature (DeMott et al, 2015; Madden and Julian, 1972, 1994; Zhang, 2005).

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