Second, for events not affected by TDPs, MJO decay over the MC occurs because weak drying, rather than moistening, is observed at MC longitudes. For these decaying events, MC drying is the result of a westward, rather than eastward, zonal gradient of MC moisture over the Equatorial MC. Both MC-crossing and MC-blocked MJO events exhibit an eastward moisture gradient just south of the MC and north of Australia—a favored location for MJO convection in many MC-crossing events. However, in decaying events, the tendency for MJO convection to split into two off-Equator gyres in the Indian Ocean leads to strong westerly wind anomalies and drying in this region, which also contribute to MJO decay.
Propagation characteristics of the MJO and TDPs in the vicinity of the MC are both consistent with moistening by horizontal winds acting on background state moisture gradients. Understanding the time and space scales of processes that alter the background moisture distribution may advance our understanding of and ability to simulate the MJO.