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Evaluating Climate Models Eric Gilleland
Research Applications Laboratory, 16th EMS Annual Meeting & 11th European Conference on
Applied Climatology, 16 September 2016 . Co-authors: Caspar Ammann, Barb Brown, Melissa Bukovsky, Seth McGinnis,
Linda Mearns, and Christopher L. Williams Support for this work provided by the NSF via the Weather and Climate Impacts Assessment Science Program (http://www.assessment.ucar.edu) and Earth System Modeling (EaSM) Grant number AGS-1243030.
UCAR Confidential and Proprietary. © 2016, University Corporation for Atmospheric Research. All rights reserved.
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Estes Park
Boulder
Fort Collins
DenverDIAGolden
NCAR/NCEP reanalysisCCSM3 Global Climate Model
Severe Storm Environments
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0.00
000
0.00
010
0.00
020
Non−severeSevereSignificant Non−tornadicSignificant Tornadic
0.00
00.
001
0.00
20.
003
0e+00 2e+05 4e+05
0.0
0.2
0.4
0.6
0.8
1.0
0 2000 6000 10000
0.0
0.2
0.4
0.6
0.8
1.0
CAPE × Shear (J kg-1 × m s-1)
Wmax × Shear (WmSh, m2 s-2)
NCEP reanalysis
Community Climate System Model
3rd Generation Coupled Global Climate Model
Hadley Centre Coupled Model, v. 3
abbreviation NCEP CCSM3 CGCM3 HadCM3
Canadian Regional Climate Model (CRCM)
X
X
X
Hadley Regional Model 3 (HRM3)
X
Pennsylvania State University/NCAR mesoscale model (MM5I)
X
X
Weather Research and Forecasting model (WRFG)
X
X
X
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http://www.narccap.ucar.edu/ http://www.emc.ncep.noaa.gov/mmb/rreanl/
Lingo
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q75: Univariate time series giving the upper quartile of a random variable (CAPE or WmSh) over space at each time point.
WmSh: As before, but set to zero if CAPE < 100 J kg-1 or 5 ≤ Shear ≤ 50 ms-1
High “field energy”: when q75 > its 90th percentile over time.
κ: Frequency of CAPE ≥ 1000 J kg-1 conditioned on the presence of high field energy.
ω: Frequency of WmSh ≥ 225 m2s-2 conditioned on the presence of high field energy.
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κ
−120 −100 −80 −70
3035
4045
NARR
−120 −100 −80 −70
3035
4045
CRCM−CCSM
−120 −100 −80 −70
3035
4045
CRCM−CGCM3
−120 −100 −80 −70
3035
4045
HRM3−HadCM3
−120 −100 −80 −70
3035
4045
MM5I−CCSM
−120 −100 −80 −70
3035
4045
MM5I−HadCM3
−120 −100 −80 −70
3035
4045
WRFG−CCSM
−120 −100 −80 −70
3035
4045
WRFG−CGCM3
−120 −100 −80 −70
3035
4045
CRCM−NCEP
−120 −100 −80 −70
3035
4045
WRFG−NCEP
020406080100
UCAR Confidential and Proprietary. © 2016, University Corporation for Atmospheric Research. All rights reserved.
ω
−120 −100 −80 −70
3035
4045
NARR
−120 −100 −80 −70
3035
4045
CRCM−CCSM
−120 −100 −80 −70
3035
4045
CRCM−CGCM3
−120 −100 −80 −70
3035
4045
HRM3−HadCM3
−120 −100 −80 −70
3035
4045
MM5I−CCSM
−120 −100 −80 −70
3035
4045
MM5I−HadCM3
−120 −100 −80 −70
3035
4045
WRFG−CCSM
−120 −100 −80 −70
3035
4045
WRFG−CGCM3
−120 −100 −80 −70
3035
4045
CRCM−NCEP
−120 −100 −80 −70
3035
4045
WRFG−NCEP
020406080100
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Image Warping
Objective Function = SSE(Warped Forecast and Observation) + Penalty term for too much bending/movement
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% error reduction ≈ 40% minimum bending energy = 2.0042
RMSE0 = 0.2665 RMSE1 = 0.1605
Image Warping
−120 −100 −90 −80 −70
3035
4045
0−energy field
0.0 0.2 0.4 0.6 0.8 1.0
−120 −100 −90 −80 −70
3035
4045
1−energy field
0.0 0.2 0.4 0.6 0.8 1.0
−120 −100 −90 −80 −70
3035
4045
Error Field
−0.8 −0.4 0.0 0.2 0.4
−120 −100 −90 −80 −70
3035
4045
Distance Travelled
5 10 15 20
−120 −100 −90 −80 −70
3035
4045
Deformed 1−energy field
0.0 0.2 0.4 0.6 0.8 1.0
−120 −100 −90 −80 −70
3035
4045
Error Field(after warping)
−0.8 −0.4 0.0 0.2 0.4
MM5I-CCSM3 κ
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Image Warping
RMSE0 RMSE1 RMSE Reduction
Minimum Bending Energy
CRCM-CCSM3 0.214 0.139 35% 0.96 CRCM-CGCM3 0.147 0.103 30% 1.07 HRM3-HadCM3 0.157 0.110 30% 0.25 MM5I-CCSM3 0.267 0.161 40% 2.00 MM5I-HadCM3 0.148 0.084 43% 0.69 WRFG-CCSM3 0.249 0.096 61% 3.27 WRFG-CGCM3 0.241 0.092 62% 3.32 CRCM-NCEP 0.214 0.173 19% 0.25 WRFG-NCEP 0.171 0.092 46% 0.43
ω results
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SPCT1 + Image Warping2 Model 1 Model 2 Mean Loss
Differential p-value
CRCM-CCSM3 MM5I-CCSM3 -1.31 0.19 HRM3—HadCM3 MM5I-CCSM3 -1.64 0.10 MM5I-CCSM3 CRCM-NCEP 1.63 0.10 MM5I-CCSM3 WRFG-NCEP 1.38 0.17 WRFG-CCSM3 CRCM-NCEP 1.76 0.08 WRFG-CCSM3 WRFG-NCEP 1.36 0.17 WRFG-CGCM3 CRCM-NCEP 1.33 0.18 WRFG-CGCM3 WRFG-NCEP 1.36 0.17
Significant results for ω at the 20% level 1See Hering and Genton (2011, Technometrics, 53 (4), 414 - 425, DOI 10.1198/TECH.2011.10136) 2See G. (2013, Mon. Wea. Rev., 141, (1), 340 – 355, DOI: 10.1175/MWR-D-12-00155.1)
10% level
ω results
Conclusions • Climate models should reproduce observed distributional properties for
the current-period climate, making spatial forecast verification methods particularly useful, and easy to implement in this context.
• Approach, here, focuses on spatial patterns of frequencies of severe-storm environments for the top ten-percent of high-energy days. § Provides a means of comparing climate models to observations without
requiring day-to-day match-ups. • Models more-or-less agree with NARR about spatial location and
overall pattern of high severe storm frequencies (κ and ω). • Models tend to under-project the spatial extent of high-frequency κ and ω areas compared to NARR.
• WRFG configurations not coupled with NCEP (i.e., “observations”) have the least agreement with NARR.
• Full analysis including many other spatial methods in G. et al. (submitted to ASCMO, available at http://www.ral.ucar.edu/staff/ericg/GillelandEtAl2016.pdf)
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