The composites and case studies indicate that the onset of the split-flow regime is dependent upon the presence of a broad, positively-tilted, trough in the South Indian Ocean, centered near 100-90°E. Equatorward fractures of cold pools from this trough help anchor a baroclinic zone over northern Australia, while the broad northwesterly flow on the east side of the trough permits a broad region of poleward warm-air advection and angular-momentum flux, enhancing the high-lati tude meridional temperature gradient and the strength of the PFJ. The split is main tained as long as incipient cyclogenesis on the front side of this trough remains relatively weak, and the cyclones propagate southeastward, poleward of broad ridge located south of Australia. However vigorous cyclogenesis in association with neu trally or negatively-tilted troughs in the South Indian Ocean results in a full-latitude and large-amplitude ridge southwest of Australia. This pattern eventually results in the creation of a strong trough downstream, generally located between 160°E to 150°W. The cold outbreaks associated with these troughs act to displace the primary meridional temperature gradient zone well equatorward, resulting in the presence of one strong, broad jet at relatively low latitudes and the absence of a split-flow regime. During the SH spring, the split-jet regime ends abruptly with a late season cold surge, after which the cold-air pool over the Antarctic land mass can not be regener ated sufficiently by radiative processes.