  With the onset of the HI Parkes All-Sky Survey, a new view of the
high-velocity cloud (HVC) distribution in the southern sky is being revealed.
The dense spatial sampling and unbiased coverage of HIPASS gives it multiple
advantages over previous surveys of the southern sky. Detailed views of the
clouds' structure and large mosaics of the HI sky allow us to link individual
concentrations to larger structures (such as the Magellanic Clouds and the
Galaxy), providing pictorial clues as to the origins of HVCs. It is clear that
HVCs cannot be uniformly assigned a single origin scenario, and must be
categorised appropriately.
