One of the main goals of PECAN is to determine whether nocturnal MCSs are elevated or surface-based and how the stable nocturnal boundary layer influences the MCS structure, evolution, and movement. A sample 4-radar analysis of the 26 June MCS at 0500 UTC (see attached image) reveals an inferred surface-based cold pool with air ascending from the surface into the updraft to form a front-to-rear (FTR) flow and a corresponding rear-to-front (RTF) flow that descends toward the surface behind and through the main reflectivity cores. Calculated Lagrangian trajectories from time-series wind analyses will reveal the source layers of air parcels (surface or elevated), allow us to determine the evolution of source levels as the MCS develops from the initial convective line to the mature MCS stage, and how radar properties of air parcels change while traversing the different sections of the MCS. Combining these 3-D airflow analyses with DLA, we will additionally infer the altitude and thermodynamic origins of updraft, downdraft, and mesoscale cold pool parcels, assess the diabatic thermodynamic forcing along selected air trajectories, derive the mesoscale cold pool depth and structure, and determine whether the MCS updrafts, downdrafts, and cold pool are elevated or surface-based.