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
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
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
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
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
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
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.
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
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
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
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
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
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 %
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
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.
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
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
SATCON Web Site
http://cimss.ssec.wisc.edu/tropic2/real-time/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
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
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
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
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
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)
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)