The sensitivity of S-Pol was maximized for LATTE by increasing the transmit power, increasing the pulse length, and increasing the number of samples. Range Height Indicator scans were made along a radial corresponding to the location of the BAO. Signals from S-Pol indicative of Bragg scatter were detected under a variety of atmospheric conditions.
Observations from S-Pol have been compared with the backscattered power recorded using the NCAR 449-MHz (67 cm) spaced antenna, multiple-frequency wind profiling radar (WPR), which was operated at the BAO during LATTE. Moreover, several radiosondes were launched from the BAO site while both S-Pol and the WPR were operating. In this presentation we discuss the theoretical framework needed to compare the relative contributions of Bragg and Rayleigh scatter for these two radars; the role of polarimetry when isolating Bragg scatter from other sources of echo power; and the implications of these findings for both research and operational atmospheric communities.
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