Handout (802.2 kB)
Preliminary results show that strong surface convergence is generally observed ahead of the front with strong surface divergence behind the front. Frontal analysis appears to be able to capture fronts that are both synoptic and mesoscale in origin and matches up well with radar imagery. There was a wide range in frequency of frontal passages throughout the mesonet with the northern and western areas observing 2-4 times the frontal passages as the southeast. The median temperature drop was 7 K while the median pressure rise was 1.5 mb. The maximum changes were 13 K and 7 mb. Only a weak correlation was found between pressure and temperature changes. This indicates that the vertical structure of the temperature perturbation in the cold pools varies from case to case. Ongoing work will entail classifying cold pools according to the properties and life-cycle stage of the convective system, determining cold pool extent and area, and applying our analysis methodology to a longer time period. The results could prove useful for evaluating the representation of cold pools in cumulus parameterizations and cloud-resolving models.