Two aspects of the 1978/79 Southern Hemisphere (SH) monsoon are examined: (i) A double-low (double-high) structure in the lower (upper) levels of the troposphere, which appears over the region adjacent to Australia; and (ii) the poleward shift in the Australian jet after the monsoon onset. Emphasis is given to the effect of the divergent circulation on these two aspects of the SH monsoon. The data generated by the FGGE IIIb analyses at the European Centre for Medium Range Weather Forecasts and the Geophysical Fluid Dynamics Laboratory are used in this study. The three-dimensional structure of the SH monsoon circulation after the monsoon onset matches well with Gill's solution based upon a heat source symmetric with respect to the equator. His solution contains the coupling of an eastward-propagating Kelvin wave and a westward-propagating mixed gravity-Rossby wave over the heat source region. Water vapor and heat budget analyses for the SH monsoon were performed to show how this heat source is maintained by the monsoon circulation. The contrast between the theories of Gill and Silva Dias et al. is discussed in order to explain the presence of the SH monsoon over the region adjacent to Australia. The poleward shift of the Australian subtropical jet stream following the SH monsoon onset is illustrated by an analysis of the energetics of the divergent and rotational flows; namely, the interaction between these two flow components and the possible adjustment of the ageostrophic circulation caused by the thermal field change after the SH monsoon onset.