steve piltz – wfo tulsa, ok don burgess – cimss norman, ok

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THE IMPACTS OF THUNDERSTORM GEOMETRY AND WSR-88D BEAM CHARACTERISTICS ON DIAGNOSING SUPERCELL TORNADOES Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

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THE IMPACTS OF THUNDERSTORM GEOMETRY AND WSR-88D BEAM CHARACTERISTICS ON DIAGNOSING SUPERCELL TORNADOES. Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK. Sidelobe Contamination. The 3D Beam (Seen on end). - PowerPoint PPT Presentation

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Page 1: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

THE IMPACTS OF THUNDERSTORM GEOMETRY AND WSR-88D BEAM CHARACTERISTICS ON

DIAGNOSING SUPERCELL TORNADOES

Steve Piltz – WFO Tulsa, OKDon Burgess – CIMSS Norman, OK

Page 2: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

The 3D Beam

(Seen on end)

Sidelobe Contamination

Page 3: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

Federal Meteorological Handbook 11- Part BDoppler Radar Theory and Meteorology

3.6 Data Contamination by Antenna Sidelobe Signal. An occasional source of datacontamination is simultaneous reception of signals at comparable power levels through both the antenna pattern main lobe and its sidelobes. This occurs when the meteorological reflectivity gradient exceeds the two-way sidelobe/main lobe isolation.

Page 4: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

27 dBTwo-way path… 27 + 27 = 54 dB

Measurements of WSR-88D radiation patters are rare. Therefore we are discussing approximations at best.

For example, if the side-lobe is sensing a 64 dBZ return, the main-beam would have to be sampling something around or less than 10 dBZ for side-lobe contamination to occur.

Page 5: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

27 dBTwo-way path… 27 + 27 = 54 dB

FMH 11: …in order to detect a signal through the first sidelobe, … the meteorological signal in the sidelobe must be stronger than the signal in the main lobe, by at least the two-way, first-sidelobe isolation. This requires a reflectivity gradient of greater than…40 dB / degree sustained over about 2 degrees. This is a rather large value and seldom-encountered in practice.

Page 6: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

NWS Training on Sidelobe Contamination

The most significant sidelobe contamination tends to occur with intense convection at close range. If the reflectivity gradients are large enough, a situation may occur where the main lobe is sampling clear air while the sidelobes are sampling the storm. In this

case, a low reflectivity would be displayed along the azimuth corresponding to the main lobe.On a reflectivity product, sidelobe contamination generally appears as a

"smearing" of low reflectivities from one azimuth to the next in a clockwise direction (The WSR-88D antenna always rotates clockwise).

Page 7: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

Which Sidelobe?

Federal Meteorological Handbook 11- Part B

Doppler Radar Theory and Meteorology

Page 8: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

Horizontal reflectivity gradients from weather targets sufficient to result in sidelobe contamination are rather rare. In the vertical they are less rare…if not common in supercells.

Vertical Reflectivity Gradients in Supercells

Page 9: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

KPAH – September 22, 2006

Page 10: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

White arrow (right):0.4 degree: -1.0 dBZ and +66 kts

Yellow arrow (right):3.3 degree: 55 dBZ and +48 kts

R X-Section

Base Vel X-Section

Page 11: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

Tornadic Meso & ??

Page 12: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

Why little / no contamination to the reflectivity?

Every -3 dB is a 50% drop of power.

Discussing power differences around -54 dB means the actual power returned is very small.

R X-Section

Base Vel X-Section

Page 13: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

But velocity data are collected. They inappropriately become a part of what the main beam samples, and the main beam’s data are contaminated.

R X-Section

Base Vel X-Section

Page 14: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

Spectrum Width

Page 15: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

Note the precision with which the Spectrum Width data “fit” into the low Reflectivity.

Page 16: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

Time Continuity

21:06 UTC

21:11 UTC

Page 17: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

Height Continuity

Page 18: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

Yellow arrow (right):1.4 degrees: -1.0 dBZ3.3 degrees: 53.0 dBZ

Base Vel X-Section

R X-Section

The 3D Beam

(Seen on end)

Page 19: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

Reflectivity 1.4 degrees21:11 UTC

Spectrum Width 1.4 degrees21:11 UTC

Page 20: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

Key Points:Vertical reflectivity gradients in the “overhang” / inflow region of supercell thunderstorms can be sufficient for sidelobe data contamination.Warning forecasters should consider the possibility of velocity contamination when the vertical reflectivity gradient is around or more than ~50 dBZ. Forecasters should closely inspect any velocity data in the inflow of supercell when the associated reflectivity is less than 25 dBZ.Contaminated velocity data will have higher associated Spectrum Width. Velocity and Spectrum Width character changes in reflectivity gradient.

Page 21: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

Needed work…The NWS should quantify the beam at each 88D in an effort to better understand this.A simple algorithm to flag areas where vertical reflectivity gradients exceed ~50 dBZ.Mesocyclone evolution needs to be studied further and training developed (Vortex2).

NWS Impacts:Warning DecisionsPathcastsAssessing Spotter Reports

Page 22: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

Future Work…

Page 23: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK
Page 24: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK
Page 25: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK
Page 26: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK
Page 27: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

Developing mesocyclone…local vorticty max…where the inflow went vertical, or ??.(Too much low-level reflectivity for sidelobe contamination.)

Page 28: Steve Piltz – WFO Tulsa, OK Don Burgess – CIMSS Norman, OK

Thank You

Steve Piltz – WFO Tulsa, OKDon Burgess – CIMSS Norman, OK