Over the tropics, two types of precipitation systems (PSs), super clusters (SCs) and Madden Julian Oscillation (MJO), are frequently observed, having similar meridionally symmetric structures about the equator but different eastward-propagating (EP) speeds. To investigate the reasons why these PSs exist, the dependence of the longitudinal variations of surface sea temperature (SST) is examined using a NICAM on an aqua-planet. In a longitudinally uniform-SST case, only SC-like fast-EP PSs appear. When the longitudinal variation of the SST increases, meanwhile, a stationary Walker circulation (WC) emerges and MJO-like slowly EP PSs occur on the western part of a high-SST area. It is expected in the real atmosphere that two different types of EP PSs can exist in parallel due to complex surface conditions: 1) SCs as free PSs and 2) MJOs as forced PSs. Here, free (forced) PSs mean convection, which is uncontrolled (controlled) by the longitudinal variation of the SST. It is also obtained that an asymmetric WC is produced, even though the SST variation symmetric about 180° longitude is forced. Owing to the WC, combined with the Hadley circulation, the MJO is generated and decayed locally, and westward-propagating PSs are dominantly observed in the subsidence areas of the WC.
IntroductionIn the tropics, organized precipitation systems (PSs) are frequently observed, such as super clusters (SCs) and Madden Julian Oscillation (MJO) (Madden and Julian 1971). Wheeler and Kiladis (1999) showed that these PSs are meridionally symmetric about the equator, but have different eastward-propagating (EP) speeds as well as horizontal scales. The SCs, which are called "Kelvin" by Wheeler and Kiladis (1999), are large-scale disturbances of zonal wave-number 2−10 with speeds of about 15−25 m s . That is, large-to planetary-scale PSs with EP speeds greater (smaller) than c c are grouped into SCs (MJOs). Our concern, then, is why two types of EP PSs, whose meridional structures are symmetric about the equator, appear or are needed.Using general circulation models, in which subgrid-scale convection is parameterized, only SC-type fast-EP disturbances were obtained in the aqua-planet, where the zonal sea surface temperature (SST) is uniform (e.g., Hayashi and Sumi 1986;Lau and Held 1988). On the other hand, MJO-like slowly EP disturbances were simulated in the longitudinally variable-SST cases (e.g., Maloney et al. 2010).Similar results were attained using a Non-hydrostatic ICosahedral Atmospheric Model (NICAM), where the microphysical process is included to explicitly represent clouds and precipitation. Multi-scale horizontal structures of SC-like fast-EP PSs with speeds of 17−20 m s −1 and mesoscale westward-propagating (WP) cloud clusters were obtained in the longitudinally uniform-SST cases (Tomita et al. 2005;Nasuno et al. 2007Nasuno et al. , 2008. In these cases, the horizontal grid size (∆) is 7 km or 3.5 km. On the other hand, using the realistic lower boundaries, such as non-uniform SST, land-sea contrast, and orography, Mi...