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Based on the appearance of band structure from the University of Miami X-band radar, all of the bands are observed to be shallow with reflectivity returns limited to below 10 km, often with a melting layer present between 4.5-5 km. Using these structures, the bands are classified into six band types: Classic (3 bands) where the convection had a clear starting and stopping point with consistent activity; Along-band (4 bands) where the band passed over the site length-wise; Lead by anvil and convection (3 bands) where the band started with low convection and an anvil before the classic structure appeared; Convection with breaks (4 bands) ; Stratiform (6 bands); and Other (3 bands). Only one of the 24 bands was not sampled by the X-band radar, and that band is excluded from classification. Initial results on the stratiform bands show a bright band just below the melting level and a peak in spectrum width in the transition region where ice and water both exist. The similarities and differences between the structures for the different band classifications will be used to explain how the band structure affects meteorological variables below the melting layer and at the surface and create a high resolution vertical mapping of rainband characteristics over land. Work is in progress to 1) characterize the vertical structure of the bands including organization, dynamics and rainfall rate; 2) study how the band passage modifies the wind and moisture fields in the boundary layer; 3) explain the melting layer processes and how they affect drop size distributions; 4) examine the momentum transports by each band; and 4) showcase the influence of the bands on surface meteorological conditions.
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