The structure and propagation of precipitation cores on a variety of c
old fronts are described. The shapes of the cores, and their orientati
ons with respect to the synoptic-scale front, are not always uniform e
ither between fronts or within the same front. Interactions between co
res depend on their proximity and relative strength. Large gaps betwee
n precipitation cores move along the cold front at a slower speed than
the cores and affect the evolution of the precipitation cores. The sp
acing of precipitation cores, the height of the head of the density cu
rrent associated with the cold front, and the strength of the cold fro
nt are positively correlated with precipitation strength. This suggest
s that interactions between cores are strongly influenced by precipita
tion. Current theories for precipitation cores on narrow cold-frontal
rainbands cannot account for these observations. A new mechanism is pr
oposed based on a positive feedback between the diabatic cooling produ
ced by the melting and evaporation of precipitation, the head of the d
ensity current, and the strength of the front.