Polarimetric Radar-Based Investigation of Microphysics in Dendritic and Needle Temperature Aggregation Zones During NASA IMPACTS

Microphysical processes that determine cloud particle habits, sizes, and concentrations can be inferred by specific polarimetric radar signatures, providing new perspectives to inform NWP models about hydrometeor types and their distributions in winter storms. In particular, areas of enhanced K DP sometimes occur in regions of aggregates within the dendritic growth zone (DGZ) and needle temperature zone (NTZ). Further, co-polar correlation coefficient (CC) reductions are sometimes found in the DGZ. These polarimetric signatures are of interest because they suggest the presence of highly nonspherical particles amongst the otherwise isotropically scattering aggregates. In this study, in-situ observations of cloud particle populations collected during the NASA IMPACTS field campaign are used to address debates in the previous literature about these signatures’ origins. In the regions of aggregates, CPI cloud particle images show a variety of particle habits that contribute to enhancing K DP or reducing CC, suggesting these polarimetric signatures may result from a combination of different particle types. Particle size, concentration, and aspect ratio data from the 2DS and HVPS probes determined that the K DP enhancement in the NTZ is produced by ice particles of 0.9-7.0-mm size, along with non-spherical aggregates with mean aspect ratio < 0.6 at sizes between 4.6-20.0 mm. Increased K DP in the DGZ is attributed to ice particles of sizes 0.4-6.0 mm. Additionally, asymmetric particles at sizes 3.0-10.0 mm are evident in the DGZ. The DGZ’s CC reduction is attributed to ice particles with sizes 1.4-5.0 mm, while CPI images show a wide range of particle types including irregularly shaped crystals that would scatter anisotropically.