| Abstract: | The structure and propagation of precipitation cores on a variety of cold fronts are described. The shapes of the cores, and their orientations with respect to the synoptic-scale front, are not always uniform either between fronts or within the same front. Interactions between cores depend on their proximity and relative strength. Large gaps between precipitation cores move along the cold front at a slower speed than the cores and affect the evolution of the precipitation cores. The spacing of precipitation cores, the height of the head of the density current associated with the cold front, and the strength of the cold front are positively correlated with precipitation strength. This suggests that interactions between cores are strongly influenced by precipitation.Current theories for precipitation cores on narrow cold-frontal rainbands cannot account for these observations. A new mechanism is proposed based on a positive feedback between the diabatic cooling produced by the melting and evaporation of precipitation, the head of the density current, and the strength of the front. |
