Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology,...

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Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma

Transcript of Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology,...

Page 1: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

Mesoscale Features of the 31 January 2011 Oklahoma Storm

Jennifer NewmanSchool of Meteorology, University of Oklahoma

Page 2: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

Event OverviewFrom 31 January to 1 February 2011, regions of thunder-sleet, freezing rain, and snow moved through Oklahoma

>100 car accidents

Close to 500 motorists stranded

4 fatalities

Page 3: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

Mesoscale FeaturesConvective activity persisted in Oklahoma, despite the fact that the atmosphere was extremely stable CSI?

Bands of snow formed in SW OK and moved throughOklahoma during the early morning of 1 February.Located ≈100 km apart Ducted gravity waves?

Page 4: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

Background: CSI

Page 5: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

Background: CSI

Page 6: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

Evaluation for CSIVertical cross-section was taken using soundings oriented along a SW-NE line. Soundings used: 00Z and 12Z 1 February 2011

Page 7: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

CSI Cross-section: 00ZPurple lines: θe

Blue lines: mg

Page 8: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

CSI Cross-section: 00ZPurple lines: θe

Blue lines: mg

CSI possible

Page 9: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

CSI Cross-section: 12ZPurple lines: θe

Blue lines: mg

Page 10: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

CSI: Brief Conclusions

Page 11: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

Background: Gravity WavesWaves are created when a boundary between materials of different densities is perturbed

-Pressure oscillations-Shifts in wind speed and direction-Vertical motion can modulate or induce precipitation

Reference: Bosart, L. F. and F. Sanders, 1986: Mesoscale structure in the Megalopolitan Snowstorm, 11–12 February 1983. Part III: A large-amplitude gravity wave. J. Atmos. Sci., 43, 924–939.

Page 12: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

Background: Ducted Gravity WavesIf a stable layer is located underneath a convectively unstable layer, gravity wave energy can be reflected and remain in the lower layer (Lindzen and Tung 1976)

Reference: Lindzen, R. S. and K.-K. Tung, 1976: Banded convective activity and ducted gravity waves. Mon. Wea. Rev., 104, 1602–1617.

Page 13: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

Mesonet Observations of Gravity Wave

Observed at all stations enclosed in red circlesData from stations in blue circles shown on next slide

Page 14: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

Mesonet Data: Pressure Oscillations

Phase speed: 28.9 m s-1

Wavelength: 200 km

Sea-Level Pressure Time Series

Pressure drop of ≈ 2-3 mb in approx. 40 minutes

Page 15: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

Ninnekah Mesonet StationSea-Level Pressure and 10-m Wind Time Series

Page 16: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

KTLX Radar: 1200 UTC

0.5° Reflectivity

Page 17: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

KTLX Radar: 1230 UTC

0.5° Reflectivity

Page 18: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

KTLX Radar: 1300 UTC

0.5° Reflectivity

Page 19: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

KTLX Radar: 1330 UTC

0.5° Reflectivity

Page 20: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

KTLX Radar: 1400 UTC

0.5° Reflectivity

Page 21: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

Mesonet vs. Radar Observations• Lowest pressure occurred just ahead of precip. band

(area of rising motion)

• From conceptual model: Greatest rising motion should occur halfway between pressure ridge and trough

• Possible that speed of precip. bands was different than phase speed of gravity wave

• Wavelength of gravity wave based on pressure fluctuations was different than wavelength of precip. bands also suggests propagation speeds were different

Page 22: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

Phase Speed Calculations

Reference: Lindzen, R. S. and K.-K. Tung, 1976: Banded convective activity and ducted gravity waves. Mon. Wea. Rev., 104, 1602–1617.

Page 23: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

Phase Speed Calculations

Page 24: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

Phase Speed Calculations

Stable layer

Unstable layer

Page 25: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

Phase Speed Calculations

Stable layer

Unstable layer

Page 26: Mesoscale Features of the 31 January 2011 Oklahoma Storm Jennifer Newman School of Meteorology, University of Oklahoma.

Summary and Conclusions• Several mesoscale features were evident from radar and satellite

imagery during the Oklahoma storm of 31 January – 1 February 2011

• Based on observed soundings, CSI was possible at low levels over Norman at 00Z 1 February - There were likely other processes occurring (frontogenesis, vorticity advection) that enhanced convection- Difficult to isolate effects of CSI

• Snow bands on 1 February appear to be associated with a gravity wave, which was observed at the surface in great detail

• Theoretical gravity wave phase speed agrees well with timing of pressure oscillations