Stratosphere-troposphere exchange (STE) is the key process regulating the flow of ozone-depleting trace gases, water vapor and other constituents into and out of the stratosphere. The overall circulation responsible for this exchange was first deduced by Brewer (1949), and it consists of upwelling in the tropics and downwelling at extratropical latitudes. This circulation is now referred to as the Brewer-Dobson circulation (BDC). Holton et al. (1995) provides a modern dynamical perspective on STE. Basically, planetary wave-breaking in the extratropical lower stratosphere drives a fluid-dynamical pump that draws air upward in the tropics and drives air downward at the pole (Haynes et al., 1991). The upward moving tropical air is forced out of radiative equilibrium, and thus the air is radiatively heated producing a net diabatic heating in the tropical upper troposphere and lower stratosphere (UTLS). Stratospheric planetary-wave breaking is most intense during winter in the Northern Hemisphere. As a result, the BDC is stronger during boreal winter and the tropical tropopause temperatures are colder than during austral winter (Yulaeva et al., 1994). Holton et al. (1995 noted that the global mass exchange rate is thus determined by the fluid-pump and not by overshooting convection or extra-tropical tropopause folding as had been previously argued.With the broad details of BDC mechanics in hand, more recent efforts have focused on the dynamics of the very lowest part of the stratosphere and the upper tropical troposphere. The BDC appears to consist of two branches: a deep branch that is forced by planetary-scale wave breaking in the mid-stratosphere (Gettelman et al., 2011;