The KSP system has recently undergone an extensive evaluation process, funded by the German EPA (the Umweltbundesamt), to determine biases and quantify model uncertainties. The present paper examines some of the key model enhancements (e.g., convective towers, eddy transport by larger eddies) and summarizes the results of comparisons with data obtained from several full-scale tracer experiments and wind tunnel studies of concentration fluctuations. This evaluation has shown that the current version of KSP:
* produces a range of ensemble -average concentration estimates that generally encompass the predictions of simple Gaussian plume models and Lagrangian particle models.
* performs similarly to simpler models in matching the crosswind-integrated and arc-maximum concentrations obtained during several tracer campaigns. This is true both for cases where most models perform well (e.g., Kincaid, Copenhagen, Prairie Grass arcs at 50m-200m) and also for cases where models generally do poorly (e.g., Lillestroem, Prairie Grass 400m-800m arcs).
* predicts a variability in concentration estimates on the order of a factor-of-two or more for tracer exposure durations of 10-60 minutes. That is, sc/C is of order unity.
* generates cumulative frequency distributions (CFDs) of concentrations that have the same qualitative behavior as those measured in the wind tunnel. These modeled CFDs are very sensitive to the assumed turbulence power spectra and its profile, nS(n,z), and assumed spectral component time scales.