In this study, we examine the evolution of NWRT PAR radial velocity to determine the effects of storm dynamics on the tornado's intensification. We also use scans from OU-PRIME and the Oklahoma City TDWR to verify velocity results using scans with greater azimuthal resolution than NWRT PAR, while WSR-88D data is used to examine tornado dissipation approximately 10 km from KTLX. With these data, we examine changes in the vertical vorticity as a function of height to determine if dynamically induced pressure perturbations impacted the tornado's intensity. We also determine how the rapid storm motion on this day may have affected locations where significant damage was observed. This analysis will allow for a better understanding of how rapid sampling and high spatial resolution may be used to detect regions of significant damage during fast-moving tornadoes.
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