| For many years, forecasters have analyzed the evolution of surface meteorological fields to gain insight into severe thunderstorm and tornado outbreaks (e.g., Miller 1972; Moller 2000). Numerous studies have shown relationships between surface features and convective initiation and organization. Structures of interest have included spatial and temporal patterns of dry line bulges (Tegtmeier 1974), low pressure systems (Tegtmeier 1974; Moller 2000), thermal and moisture ridges (Miller 1972; Moller 1979), and outflow boundaries (Markowski et al. 1998a). Outflow boundaries may be determined directly by the means of mesoscale surface analysis, or inferred by noting where the WSR-88D accumulated precipitation algorithm indicates that previous storms have laid down a swath of soil-wetting precipitation (Markowski et al. 1998a). Frequently more than one of the favored features is present and it becomes an enormous challenge for the forecaster to decide which features will trigger convection and which will influence the evolution of the thunderstorms. As one might expect May 3, 1999 was no exception. A moist, unstable boundary layer, a dry line and other surface boundaries, and vertical wind shear favorable for supercells covered a large geographic area. Were there clues in the surface fields that might have suggested the location of convective initiation and convective mode? The surface features in this event were well sampled in both the traditional synoptic scale data sets and in the Oklahoma Mesonet. Four analyses of traditional fields were conducted; a manual analysis of the synoptic data, a manual analysis supplemented by mesonet data, an objective analysis of the synoptic data, and an objective analysis supplemented by mesonet data. Aspects of the four analyses are compared. |