The Walker circulation is the most prominent planetary-scale tropical atmospheric circulation in the zonal direction (e.g., Bjerknes, 1969;Walker, 1923Walker, , 1924. It has been understood that, to first order, the vertical motion associated with the Walker circulation consists of upward branches over relatively warm surfaces (e.g., the warm pool in the western Pacific) and downward branches over relatively cool surface (e.g., the cold tongue in the eastern Pacific; e.g., Lau & Yang, 2003). In the context of climate variability, trends and interannual variability of the Walker circulation have long been investigated in association with climate modes and the greenhouse gas forcing (e.g., Tanaka et al., 2004). In particular, the Pacific branches of the Walker circulation have received much attention, because its interannual fluctuation serves as the atmospheric component of the El Niño Southern Oscillation (ENSO), the most dominant interannual climate mode on Earth (e.g., Bjerknes, 1969).As a mean state, however, a downward branch of the Walker circulation above the western Indian Ocean also exhibits a strong subsidence, which is at least comparable to the Pacific downward branch. Figure 1a shows the annual-mean equatorial vertical motion calculated by taking the meridional mean over the