To complete this research goal, archived radar were analyzed for the months of May through September over a ten year span to identify cases of mesoscale convective systems interacting with the Black Hills. The criteria for the ~250 cases was, at some time during transition over the Black Hills, had to have a maximum reflectivity of at least 40 dbz, and had to have a width-to-length ratio of at least 1 to 3. As long as the line obtained these criteria at some point in its transition, it is allowed to decrease in intensity to a smaller/weaker system, or even dissipate completely, and still be considered as a case. Each case was then divided into three time periods: upstream from the hills, crossing the hills, and downstream from the hills. Within each of these partitioned zones, the cases were manually categorized based on a dominant convective modes as Single Cell, Multiple Cells, Width-to-length ratios of 1 to 2 or 1 to 3, and Long.
This presentation will detail the classification of these cases, and further quantify changes in intensity as MCSs encounter the Black Hills using plots of maximum reflectivity accumulated over time. Changes in intensity will also be compared with changes to the background environmental conditions with an aim toward isolating terrain effects from the MCS responding to environmental heterogeneity. Ultimately, through improved understanding of the interactions between MCSs and underlaying terrain, this research aims to further improve short-term forecasts of MCSs and their associated severe weather.