Title: Phased Array Radar
1 Comparison of Storm Evolution Characteristics
NWRT and WSR-88D
What are the benefits and challenges of using a
Phased Array Antenna for meteorological
surveillance?
33rd International Conference
on Radar Meteorology 7 August 2007
Pam Heinselman David
Priegnitz, Kevin Manross, Travis Smith, Rick
Hluchan OU CIMMS / NSSL
2Advantage of NWRT Phased Array Radar Faster Scan
Rates
Ultimate Goal
What we have now
3Advantage of NWRT Phased Array Radar Adaptable
Scan Capability
Radar Control Interface with VCP selector open
4Phased Array Radar WSR-88D
Comparison
Similarities
Wavelength (9.4 cm) Range Resolution (250
m) Can mimic WSR-88D VCPs
5Earlier confirmation of intensifying/contracting
gust front
223346 UTC
24 April 2006
PAR VCP 12 clone 90? sector
Images 58 s
WSR-88D VCP 12
Images 4.1 min
6Earlier confirmation of
reintensifying supercell
223346 UTC
Max vorticity gt .0075 s-1
7Better coherence
in circulations
PAR
PAR
PAR VCP 12 clone
45? sector Images 30 s
KTLX
KTLX
WSR-88D VCP 12
Images 4.1 min
8Earlier detection of
tornadic vortex signature
PAR
PAR
Union City, OK Tornado (5/9/07)
PAR VCP 12 clone
45? sector Images 30 s
KTLX
KTLX
WSR-88D VCP 12
Images 4.1 min
9Earlier detection of large hail aloft
223346 UTC
15 August 2006
PAR Reflectivity cross-section, cappi (10 km),
and 0.5? PPI 31 elevation scans up
to 41?, 831 ?s PRT 90? sector
Images 26 s
Simulated WSR-88D Reflectivity cross-section,
cappi (10 km), and 0.5? PPI Images 5 min
10Earlier detection of microburst
223346 UTC
10 July 2006
PAR VCP 12 clone 90? sector
Images 34 s
WSR-88D VCP 12
Images 4.1 min
11PAR Benefits Challenges
- Allows focus on high-impact events
- More timely data interpretation
decision-making - Improved confidence in feature location,
intensity, and evolution - Potential to improve algorithm performance
- Choosing sector location
- Cognitive overload
- Understanding small-scale transient phenomena
that are not observed regularly in WSR-88D data - Radar hardware and display software limitations