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