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This presentation by Mike Dixon, John Hubbert, Greg Meymaris, and Scott Ellis examines improvements in Clutter Mitigation Decision (CMD) techniques, focusing on single polarization radar data analysis. Key topics include phasor diagrams, case studies from KEMX and KFTG, and the impact of clutter on reflectivity measurements. The findings show that modifications to the Clutter Profile Algorithm (CPA) can yield higher and smoother results for both clutter and weather detection. Ongoing tuning and testing are recommended to optimize these enhancements.
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CLUTTER MITIGATION DECISION (CMD)INVESTIGATION OF IMPROVEMENTSFOR SINGLE POLARIZATION CMD Mike Dixon, John Hubbert, Greg Meymaris and Scott EllisNational Center for Atmospheric ResearchBoulder, Colorado Technical Interchange Meeting for NEXRAD enhancementsROC, NSSL, NCAR Boulder, CO June 2010
Presentation overview • Phasor diagrams • KEMX example • KFTG low-angle tilt • KFTG high-angle tilt
KEMX – clutter - original vs. modified CPA Original CPA Modified CPA
KEMX – clutter - original vs. modified CPA Original CPA Modified CPA
KEMX – Reflectivity DBZ DBZ Filtered
KEMX – TDBZ and SPIN TDBZ SPIN
KEMX – CPA and CMD flag New CPA CMD flag
Conclusion – Improved CPA needs tuning and testing • Method: compute CPA using some fraction of the parts which yield a maximum value. • This leads to higher values of CPA and a generally smoother result. • In addition to being smoother, this version of CPA shows higher values in both clutter and weather. • Therefore, further tuning and testing is required.