Three separate techniques are used to document the mesoscale features of wave and frontal structures within the comma head region of the 15 and 22 February 2010 cyclones. The first incorporates radial velocity measurements from both the nadir and slanted beams of the WCR to conduct a dual-Doppler synthesis that details the flow structures within the cloud. Another technique uses velocity measurements from the WCR slant beam to depict isentropic surfaces and other notable structures at a very fine resolution. Lastly, RHI scans from the X-band radar are used to determine any additional structures that may be present within this region of the cyclone, and their relationship to radar signatures in dual-polarization features.
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