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TC Intensity Estimation: SATellite CONsensus (SATCON)

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TC Intensity Estimation: SATellite CONsensus (SATCON). University of Wisconsin - Madison Cooperative Institute for Meteorological Satellite Studies. Derrick Herndon and Chris Velden. Interdepartmental Hurricane Conference Savannah, GA 01-04 March 2010. Research supported by - PowerPoint PPT Presentation
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TC Intensity Estimation: TC Intensity Estimation: SATellite CONsensus (SATCON) SATellite CONsensus (SATCON) Derrick Herndon and Chris Velden Interdepartmental Hurricane Conference Interdepartmental Hurricane Conference Savannah, GA Savannah, GA 01-04 March 2010 01-04 March 2010 Research supported by the ONR Marine Meteorology and Atmospheric Effects Program University of Wisconsin - Madison Cooperative Institute for Meteorological Satellite Studies
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Page 1: TC Intensity Estimation: SATellite CONsensus (SATCON)

TC Intensity Estimation: SATellite TC Intensity Estimation: SATellite CONsensus (SATCON)CONsensus (SATCON)

Derrick Herndon and Chris Velden

Interdepartmental Hurricane ConferenceInterdepartmental Hurricane ConferenceSavannah, GASavannah, GA

01-04 March 201001-04 March 2010

Research supported by the ONR Marine Meteorology and Atmospheric Effects Program

University of Wisconsin - Madison

Cooperative Institute for Meteorological Satellite Studies

Page 2: TC Intensity Estimation: SATellite CONsensus (SATCON)

Motivation• Importance of getting current TC intensity right

- Intensification trends > forecasts- Predictor for statistical forecast models- Climatology (Basin Best Tracks)- Initial conditions for numerical models

• Contemporary methods to estimate TC intensity can vary by more than 40 knots

• Several objective TC intensity methods exist, but the goal of SATCON is to assist forecasters in assessing current intensity by combining the confident aspects of the individual objective estimates into a single “best” estimate

Page 3: TC Intensity Estimation: SATellite CONsensus (SATCON)

MotivationRecon vs Dvorak for 15W (MSW)

30

40

50

60

70

80

90

100

110

120

130

140

6:00 6:00 8:00 12:00 18:00 5:00 4:00 18:00 7:00

9-Sep 10-Sep 10-Sep 11-Sep 12-Sep 18-Sep 19-Sep 19-Sep 20-Sep

B1 B5 B3 B4 B2

Page 4: TC Intensity Estimation: SATellite CONsensus (SATCON)

MotivationRecon vs Dvorak for 15W (MSW)

30

40

50

60

70

80

90

100

110

120

130

140

6:00 6:00 8:00 12:00 18:00 5:00 4:00 18:00 7:00

9-Sep 10-Sep 10-Sep 11-Sep 12-Sep 18-Sep 19-Sep 19-Sep 20-Sep

Recon B1 B5 B3 B4 B2 Blind Mean

Page 5: TC Intensity Estimation: SATellite CONsensus (SATCON)

SATCON MembersADT (Advanced Dvorak Technique)

Uses IR imagery to objectively assess storm cloud patterns and structure to infer intensity

Latest version uses information from MW to make adjustments

Clear Eye Pinhole Eye Large Eye

ShearCurved Band Uniform

Page 6: TC Intensity Estimation: SATellite CONsensus (SATCON)

SATCON Members: CIMSS AMSU

0

20

40

60

80

100

120

-1 0 1 2 3 4 5 6 7 8

Channel 6

Channel 7

Channel 8

350 mb

250 mb

150 mb

AMSU Tb Anomaly vertical cross section for Katrina 2005

70 Knots

125 knots

55 Knots

AMSU Channel 8 Tb Anomaly Magnitude

TC

Pre

ssur

e A

nom

aly

Mag

nitu

de

Page 7: TC Intensity Estimation: SATellite CONsensus (SATCON)

SATCON Members: CIRA AMSU

IR image from NRL TC Page

AMSU-A Tb are used to produce a statistical temperature retrieval at 23 pressure levels. Estimates of Vmax are then determined from the thermal warm core structure.

Page 8: TC Intensity Estimation: SATellite CONsensus (SATCON)

SATCON

The strengths and weaknesses of each method are assessed based on statistical analysis, and that knowledge is used to assign weights to each method in the

consensus algorithm based on situational performance to arrive at a single intensity

estimate

Page 9: TC Intensity Estimation: SATellite CONsensus (SATCON)

Another component of SATCON is cross-method information sharing

• What relationships might exist between the parameters of the member algorithms?

• Can some of the unique information from these parameters be shared between the algorithms to improve the individual members?

• Corrections can be made to improve the performance of each algorithm, then the weights re-derived to produce an improved weighted consensus

Page 10: TC Intensity Estimation: SATellite CONsensus (SATCON)

Adjust AMSU pressure if

needed

SATCON cross-method information sharing

ADT Estimate of Eye Size

Compare to AMSU-A FOV resolution

Example: ADT to AMSU

In eye scenes, IR can be used to estimate eye size

CIMSS AMSU uses eye size information to correctresolution sub-sampling

Page 11: TC Intensity Estimation: SATellite CONsensus (SATCON)

Example: Objective estimates of eye size from CIMSS ‘ARCHER’ method (using MW imagery)

Currently, AMSU uses IR-based eye size or values from op center if no eye in IR.

MW imagery (MI) often depicts eyes when IR/ADT cannot

ARCHER method (Wimmers and Velden, 2010) uses objective analysis of MI and accounts for eyewall slope

Information Sharing

ARCHER eye = 33 km Information can be input to AMSUmethod

Page 12: TC Intensity Estimation: SATellite CONsensus (SATCON)

SATCON Weighting Scheme

Example: ADT Scene type vs. performance

Weights are based on situational analysis for each member• Separate weights for MSW and MSLP estimates• Example criteria: scene type (ADT) scan geometry/sub-sampling (AMSU)

RMSE 14 knots RMSE 12 knots RMSE 18 knots

CDO EYE SHEAR

Page 13: TC Intensity Estimation: SATellite CONsensus (SATCON)

Examples

ADT determines scene is an EYE

CIMSS AMSU: Good, near nadir pass. Eye is well resolved by AMSU resolution

CIRA is sub-sampled by FOV offset with TC center

SATCON Weighting:ADT = 28 % CIMSS AMSU =47 % CIRA AMSU = 25 %

Page 14: TC Intensity Estimation: SATellite CONsensus (SATCON)

Examples

ADT determines scene is a SHEAR scene

CIMSS AMSU indicates no sub-sampling present

CIRA AMSU: little sub-sampling due to position offset from FOV center

SATCON Weighting:ADT = 18 % CIMSS AMSU =41 % CIRA AMSU = 41 %

Center of TS Chris

Page 15: TC Intensity Estimation: SATellite CONsensus (SATCON)

1999-2009 performance stats (Vmax) - Atlantic

N = 460N = 460CIMSSCIMSS

AMSUAMSU

CIMSSCIMSS

ADTADTCIRA CIRA AMSUAMSU

SATCONSATCON

BIASBIAS 4.04.0 - 5.0- 5.0 -8.6-8.6 -1.0-1.0

AVG AVG ERRORERROR 9.19.1 11.511.5 12.312.3 7.27.2

RMSERMSE 10.210.2 13.513.5 14.614.6 8.38.3

Dependent sample. Values in knots. Validation is best track Vmax coincident with aircraft recon +/- 3 hours from estimate time. Negative bias = method was too weak.

Page 16: TC Intensity Estimation: SATellite CONsensus (SATCON)

1999-2009 SATCON compared to a simple straight consensus (Atlantic)

N = 460N = 460SATCONSATCON

MSLPMSLP

SIMPLESIMPLE

MSLPMSLPSATCON SATCON

VmaxVmaxSIMPLESIMPLE

VmaxVmax

BIASBIAS 0.30.3 -2.5-2.5 -1.0-1.0 - 4.0- 4.0

AVG AVG ERRORERROR 5.25.2 5.75.7 7.27.2 8.18.1

RMSERMSE 6.46.4 7.77.7 8.38.3 9.39.3

Dependent sample. Vmax validation in knots vs. BT. MSLP validation in hPa vs. recon. Negative bias = method was too weak. SIMPLE is simple average of the 3 members

Page 17: TC Intensity Estimation: SATellite CONsensus (SATCON)

1999-2009 SATCON compared to operational Dvorak (Atlantic)

N = 460SATCON

MSLP

Dvorak

MSLPSATCON

VmaxDvorak

Vmax

BIAS 0.3 -2.7 -1.0 -3.0

AVG ERROR

5.2 7.6 7.2 8.1

RMSE 6.4 9.1 8.3 9.0

Dependent sample. Vmax validation in knots vs. BT. MSLP validation in hPa vs. recon. Neg. bias = method was too weak. Dvorak is average of TAFB and SAB estimates

Page 18: TC Intensity Estimation: SATellite CONsensus (SATCON)

SATCON Web Site

http://cimss.ssec.wisc.edu/tropic2/real-time/satcon

Page 19: TC Intensity Estimation: SATellite CONsensus (SATCON)

A weighted consensus of three objective satellite-based methods to estimate TC intensity (SATCON) shows skill compared to conventional Dvorak-based methods.

Independent trials during 2008 and 2009 in the Atlantic support the dependent sample results.

SATCON also showed skill vs. other methods in the WestPac during TPARC/TCS-08 in 2008 (small sample of validated cases).

SATCON is run experimentally on all global TCs in real-time, with the information available on the CIMSS TC web site.

Summary

Page 20: TC Intensity Estimation: SATellite CONsensus (SATCON)

Brueske K. and C. Velden 2003: Satellite-Based Tropical Cyclone Intensity Estimation Using the NOAA-KLM Series Advanced Microwave Sounding Unit (AMSU). Monthly Weather Review Volume 131, Issue 4 (April 2003) pp. 687–697

Demuth J. and M. DeMaria, 2004: Evaluation of Advanced Microwave Sounding Unit Tropical-Cyclone Intensity and Size Estimation Algorithms. Journal of Applied Meteorology Volume 43, Issue 2 (February 2004) pp. 282–296

Herndon D. and C. Velden, 2004: Upgrades to the UW-CIMSS AMSU-based TC intensity algorithm.Preprints, 26th Conference on Hurricanes and Tropical Meteorology, Miami, FL, Amer. Meteor. Soc., 118-119

Olander T. and C. Velden 2007: The Advanced Dvorak Technique: Continued Development of an Objective Scheme to Estimate Tropical Cyclone Intensity Using Geostationary Infrared Satellite Imagery. Wea. and Forecasting Volume 22, Issue 2 (April 2007) pp. 287–298

Velden C. et al., 2006: The Dvorak Tropical Cyclone Intensity Estimation Technique: A Satellite-Based Method that Has Endured for over 30 Years. Bulletin of the American Meteorological Society Volume 87, Issue 9 (September 2006) pp. 1195–1210

Wimmers, A., and C. Velden, 2010: Objectively determining the rotational center of tropical cyclones in passive microwave satellite imagery. Submitted to JAMC.

References

Page 21: TC Intensity Estimation: SATellite CONsensus (SATCON)

ISABEL 2004 VMAX

70

80

90

100

110

120

130

140

150

17:00 2:00 18:00 23:00 7:00 11:00 18:00 22:00 2:00 7:00 15:00 18:00 2:00 6:00 23:00 12:00

12-Sep 13-Sep 14-Sep 14-Sep 15-Sep 15-Sep 15-Sep 15-Sep 16-Sep 16-Sep 16-Sep 16-Sep 17-Sep 17-Sep 17-Sep 18-Sep

Vmax (knots)

Recon SATCON DVK

Page 22: TC Intensity Estimation: SATellite CONsensus (SATCON)

KATRINA 2005 Vmax

20

40

60

80

100

120

140

160

8:00 19:00 11:00 11:00 20:00 8:00 12:00 20:00 8:00 12:00

24-Aug 24-Aug 25-Aug 26-Aug 27-Aug 28-Aug 28-Aug 28-Aug 29-Aug 29-Aug

Vmax (knots)

Recon SATCON Dvorak

Page 23: TC Intensity Estimation: SATellite CONsensus (SATCON)

WILMA 2005 Vmax

0

20

40

60

80

100

120

140

160

180

11:00 20:00 23:00 9:00 11:00 20:00 8:00 11:00 20:00 23:00 19:00 22:00 7:00 11:00

16-Oct 18-Oct 18-Oct 19-Oct 19-Oct 19-Oct 20-Oct 20-Oct 20-Oct 22-Oct 24-Oct 24-Oct 25-Oct 25-Oct

Vmax (knots)

Recon SATCON Dvorak

Page 24: TC Intensity Estimation: SATellite CONsensus (SATCON)

Analysis of Sat-Based TC Intensity Analysis of Sat-Based TC Intensity Estimation in the WNP During TCS-08Estimation in the WNP During TCS-08

N=14

‘Blind’

DvorakConsensus

OperDvorakConsensus

(w/Koba)

ADTw/MW

CIMSSAMSU

SATCON

Bias 3.6 2.0 -3.6 2.9 -0.1

Abs Error

9.3 12.0 13.6 8.6 9.0

RMSE 11.9 14.9 17.4 10.1 10.6

Positive Bias indicates method estimates are too strong

Comparison of All Satellite-based Estimates – Vmax (Kts)

Page 25: TC Intensity Estimation: SATellite CONsensus (SATCON)

Analysis of Sat-Based TC Intensity Analysis of Sat-Based TC Intensity Estimation in the WNP During TCS-08Estimation in the WNP During TCS-08

N=14

‘Blind’

DvorakConsensus

OperDvorakConsensus

(w/Koba)

ADTw/MW

CIMSSAMSU

SATCON

Bias 0.7 0.1 -1.0 -1.9 -1.3

Abs Error

5.2 7.5 10.7 4.9 6.0

RMSE 6.6 8.9 12.8 6.3 7.2

Positive Bias indicates method estimates are too strong. 2mem SATCON RMSE= 4.7Blind and Oper Dvorak conversion is Knaff/Zehr

Comparison of All Satellite-based Estimates – MSLP (mb)


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