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An Investigation of Model-Simulated Band Placement and Evolution in the 25 December 2002 Northeast U.S. Banded Snowstorm David Novak NOAA/ NWS Eastern Region Headquarters, Scientific Services Division, Bohemia, New York Stony Stony Brook University, State University of New York, Stony Brook, New York Brian Colle Stony Brook University, State University of New York, Stony Brook, New York Daniel Keyser University at Albany, State University of New York, Albany, New York

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An Investigation of Model-Simulated Band Placement and Evolution in the 25 December 2002 Northeast U.S. Banded Snowstorm. David Novak - PowerPoint PPT Presentation

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Page 1: David Novak

An Investigation of Model-Simulated Band Placement and Evolution in the 25 December 2002 Northeast

U.S. Banded Snowstorm

David NovakNOAA/ NWS Eastern Region Headquarters, Scientific Services Division, Bohemia, New York Stony

Stony Brook University, State University of New York, Stony Brook, New York

Brian ColleStony Brook University, State University of New York, Stony Brook, New York

Daniel KeyserUniversity at Albany, State University of New York, Albany, New York

Page 2: David Novak

Previous WorkCompare Eta, MM5, and WRF forecasts to observations

– Models initialized with EDAS

at 0000 UTC 25 Dec 2002

– 36/12/4 km one-way nest

for MM5/WRF

Model SST Convection PBL Micro-physics

Eta Eta BMJ MYJ Ferrier

MM5 v3.4.0

Navy Grell MRF Simple Ice (3 class)

WRF v2.0.3

Navy Grell–Devenyi MRF WSM-3

Page 3: David Novak

MSLP Time Series

MSLP Time Series

960

965

970

975

980

985

990

995

1000

12Z 15Z 18Z 21Z 00Z 03Z 06Z

Time (UTC)

MS

LP

(m

b) Obs

Eta

MM5

WRF

Page 4: David Novak

12 km MM5 12 km WRF

•Simulated Radar Reflectivity (shaded, dBZ)

•700-hPa height (thick solid, m)

•700-hPa 2D Miller Frontogenesis (thin solid, °C 100 km-1 h-1)

1800 UTC

Page 5: David Novak

12 km MM5 12 km WRF

•Simulated Radar Reflectivity (shaded, dBZ)

•700-hPa height (thick solid, m)

•700-hPa 2D Miller Frontogenesis (thin solid, °C 100 km-1 h-1)

2000 UTC

Page 6: David Novak

12 km MM5 12 km WRF

•Simulated Radar Reflectivity (shaded, dBZ)

•700-hPa height (thick solid, m)

•700-hPa 2D Miller Frontogenesis (thin solid, °C 100 km-1 h-1)

2200 UTC

Page 7: David Novak

12 km MM5 12 km WRF

•Simulated Radar Reflectivity (shaded, dBZ)

•700-hPa height (thick solid, m)

•700-hPa 2D Miller Frontogenesis (thin solid, °C 100 km-1 h-1)

0000 UTC

Page 8: David Novak

4 km MM5 4 km WRF

•700-hPa 2D Miller Frontogenesis (shaded, °C 100 km -1 h-1)

•700-hPa temperature (thick solid, C)

•700-hPa wind barbs

2000 UTC

Page 9: David Novak

Motivation• Why did the MM5 and WRF models forecast the

band too far to the southeast?– Is the deformation/frontogenesis farther northwest?

• Can the modeled sharp 700-hPa trough and attendant intense frontogenesis be verified?

• What accounts for the different band evolution forecasts in the WRF and MM5?– MM5: one single band that dissipates early– WRF: correct event length but two separate bands

Page 10: David Novak

Analyses and Observations

• RUC and EDAS used for analysis, with supplemental tropospheric observations

Datasource Variables Instrument Error

NOAA Profiles Wind 1 kt; 3 degrees

WSR-88D VAD Wind Situationally dependent

MDCRS Wind, Temp 3–5 kt, 5 degrees

Analysis Resolution Technique

RUC 20 km OI

EDAS 12 km 3-D VAR

Page 11: David Novak

Analyses and Observations18 UTC

RUC

700 mb Height (red, 15 m)

700 mb Temp (shaded, 2°C)

Analysis Winds (white barb)

Observed Winds (black barb)

Page 12: David Novak

RUC vs. EDAS18 UTC

RUCEDAS

Page 13: David Novak

Analyses and Observations19 UTC

RUC

700 mb Frontogenesis (red, °C 100 km-1 h-1)

700 mb Temp (shaded, 2°C)

Analysis Winds (white barb)

Observed Winds (black barb)

Page 14: David Novak

Analyses and Observations22 UTC

RUC

700 mb Frontogenesis (red, °C 100 km-1 h-1)

700 mb Temp (shaded, 2°C)

Analysis Winds (white barb)

Observed Winds (black barb)

Page 15: David Novak

Analyses and Observations00 UTC

RUC

700 mb Frontogenesis (red, °C 100 km-1 h-1)

700 mb Temp (shaded, 2°C)

Analysis Winds (white barb)

Observed Winds (black barb)

Page 16: David Novak

RUC vs. EDAS00 UTC

RUCEDAS

Page 17: David Novak

MM5 and WRF19 UTC

WRFMM5

Page 18: David Novak

MM5 and WRF22 UTC

WRFMM5

Page 19: David Novak

MM5 and WRF01 UTC

WRFMM5

Page 20: David Novak

Features of Note

• Sharp 700-hPa trough, attendant winds and frontogenesis can be verified

• Trough and associated frontogenesis farther northwest than models forecast

• Easterly flow forecast in WRF run over CT was not observed

Page 21: David Novak

p

fgPV )(

Potential Vorticity

• High values of PV associated with– Cyclonic flow

– High static stability

– Low tropopause

– Upper trough

• Low values of PV associated with– Anticyclonic flow

– Low static stability

– High tropopause

– Upper ridge

• PV is the product of the – Absolute vorticity

– Static stability

Figures from Thorpe (1985) for Northern Hemisphere

Slide courtesy Dr. Mike Brennen (NCSU)

Page 22: David Novak

Dynamic Tropopause12 UTC

MM5 WRF

Pressure and winds on the PV=2 PVU surface (shaded)

Page 23: David Novak

Dynamic Tropopause15 UTC

MM5 WRF

Page 24: David Novak

Dynamic Tropopause16 UTC

MM5 WRF

Page 25: David Novak

Dynamic Tropopause17 UTC

MM5 WRF

Page 26: David Novak

Dynamic Tropopause18 UTC

MM5 WRF

Page 27: David Novak

Dynamic Tropopause19 UTC

MM5 WRF

Page 28: David Novak

Dynamic Tropopause20 UTC

MM5 WRF

Page 29: David Novak

Dynamic Tropopause21 UTC

MM5 WRF

Page 30: David Novak

Dynamic Tropopause22 UTC

MM5 WRF

Page 31: David Novak

Dynamic Tropopause23 UTC

MM5 WRF

Page 32: David Novak

Dynamic Tropopause00 UTC

MM5 WRF

Page 33: David Novak

Dynamic Tropopause01 UTC

MM5 WRF

Page 34: David Novak

Dynamic Tropopause02 UTC

MM5 WRF

Page 35: David Novak

• PV generated below level of maximum heating – Warming increases static stability– Pressure falls convergence increases absolute vorticity

PV+PV+

PV-PV-

PV and Latent HeatingPV and Latent Heating

• Opposite occurs above level of maximum heating where PV is reduced

• PV growth rate determined by vertical gradient of LHR

Slide courtesy Dr. Mike Brennen (NCSU)

Page 36: David Novak

12 UTCModel PV - Reflectivity Comparison

MM5 WRF

Pressure/winds on the DT (shaded) and reflectivity contoured > 32 dBZ

Page 37: David Novak

15 UTCModel PV - Reflectivity Comparison

MM5 WRF

Page 38: David Novak

16 UTCModel PV - Reflectivity Comparison

MM5 WRF

Page 39: David Novak

17 UTCModel PV - Reflectivity Comparison

MM5 WRF

Page 40: David Novak

18 UTCModel PV - Reflectivity Comparison

MM5 WRF

Page 41: David Novak

19 UTCModel PV - Reflectivity Comparison

MM5 WRF

Page 42: David Novak

20 UTCModel PV - Reflectivity Comparison

MM5 WRF

Page 43: David Novak

21 UTCModel PV - Reflectivity Comparison

MM5 WRF

Page 44: David Novak

22 UTCModel PV - Reflectivity Comparison

MM5 WRF

Page 45: David Novak

23 UTCModel PV - Reflectivity Comparison

MM5 WRF

Page 46: David Novak

00 UTCModel PV - Reflectivity Comparison

MM5 WRF

Page 47: David Novak

PV Cross Sections21 UTC

MM5 WRF

Page 48: David Novak

800-600 mb PV21 UTC

MM5 WRF

Page 49: David Novak

PV Findings• Model-simulated bands appear downwind of

PV filaments

• PV filaments appear to be created by diabatic processes occurring in southeast sector of cyclone

• Simulated band evolution was particularly sensitive to diabatically-generated lower-tropospheric PV anomaly over Long Island

Page 50: David Novak

Conclusions and Implications

•Southeast band position error appears to be due to a misplacement of the sharp 700-hPa trough and associated frontogenesis

•Although both the MM5 and WRF successfully predicted band formation, respective band evolution appears to be sensitive to convection occurring in the southeast sector of the cyclone

• Suggests the likelihood of banding may be more predictable than exact timing, location, and evolution

Page 51: David Novak

18 UTCRadar Observations

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19 UTCRadar Observations

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20 UTCRadar Observations

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21 UTCRadar Observations

Page 55: David Novak

22 UTCRadar Observations