Of particular interest are data collected on 10 November 2018. RELAMPAGO mobile radars and other surface assets sampled a supercell, which produced a short-lived tornado-scale vortex. This vortex was sub-tornadic in strength (delta-V < 40 m s-1) and, although it formed within a supercell, its genesis mechanism may have been more typical of non-supercell tornadoes. Large hail was observed in the domain. Dual-Doppler data between 1920 UTC and 2030 UTC from the DOW 6 and DOW 7 mobile X-band radars captured much of the tornado-scale vortex genesis and evolution. Frequent, proximate soundings allow for assessment of the near-storm environment. Surface weather stations and mobile mesonets provided further information about the near-storm environment and storm-generated boundaries. In addition to kinematic and dual-Doppler analyses, the dual-pol products from DOWs 6 and 7 allow for assessment of the microphysical evolution and associated mesoscale processes that may have contributed to vortex genesis. DOW6, for the first time, operated in simultaneous LDR and fast-45 mode and may provide additional microphysical insights regarding storm structure and evolution.
Preliminary analyses suggest a complicated genesis of the tornado-scale vortex, as it formed in a region where the storm-generated gust front interacted with linear environmental boundary layer features. Although preliminary proximal environmental soundings suggest the low-level shear was sufficient for supercells, preliminary analysis of the DOW radar data suggest that the shear associated with the storm-generated cold pools exceeded the environmental shear. We will discuss our initial findings, including the storm structure, updraft/downdraft and microphysical evolution, and the interaction of the storm with its environment, as well as how this storm fits into the spectrum of storms and pre-convective environments observed during the RELAMPAGO field campaign.