medeiros poster nasa pmm 2019...medeiros_poster_nasa_pmm_2019 created date: 10/30/2019 3:28:40 pm
TRANSCRIPT
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Identifying Extreme Precipitation in GPMfor Evaluating Climate ModelsBrian Medeiros, Kevin Reed, Erica Bower, Angeline Pendergrass, Julie Caron
Total annual meanprecipitation [mm/yr] (left),annual mean precipitationfrom Tropical Cyclones (TC)[mm/yr] (middle), andpercentage of the annualmean precipitation that isdue to TCs (right). Uppertwo rows showobservations, 3rd row is ahigh-resolution CESM1simulation (similar toHighResMIP models), 4throw is a low-resolutionCESM1 simulation (similar toCMIP models).
Annual maximum 5-dayaccumulated precipitation
(Rx5day) [mm/yr] (left),TC-related Rx5day
[mm/yr] (middle), andpercentage of Rx5day
events due to TCs (right).
OrganizedSystemsrole inclimatology
OrganizedSystemsrole in
extremes
Identify organized precipitation events from the GPM andTRMM products using a precipitation-focused approach
Classify organized precipitation events based on overlapbetween precipitation- and dynamically-based trackingalgorithms
Confront standard- and high-resolution models withobservations of organized precipitation
What are the characteristics of convective organization, includingfrequency, duration, location and spatial extent as observed bysatellites? How do organized events, including extreme forms ofweather, contribute to the probability distribution of precipitation,especially its extreme tail?
How are extreme precipitation events related to dynamically-driven weather phenomena?
Do high-resolution climate model simulations capture theobserved relationships between extreme precipitation andorganized convection better than conventional-resolutionsimulations?
TASKSQUESTIONS
non-
MCSP
recip
itatio
nMC
SPrecip
itatio
n PRESENT (1991-2005) FUTURE (2070-2099)
mm d-180°W100°W120°W80°W100°W120°W
30°N
40°N
50°N
30°N
20°N
40°N
50°N8
20
46
24
6
0
12
18
Composite May precipitation from CESM1 at 0.25°,separately for Mesoscale Convective Systems (MCS), andother. On the left is present, and on the right is a projectionof the late 21st Century.
High-resolution models
60
1 10−60
−30
0
30
1 10 1 10 100 0
0.05
0.1
0.15
0.2GPCP GPM TRMM
Three views of observed rain distributions. Note GPM &TRMM both have rain rates >50 mm d-1, while GPCPdoes not.
Contrast the observed rain distribution with CMIP5models. Most of these models have grid spacing around100 km. There is a large diversity among models, withmost being skewed toward lighter rain rates. Is this biasbecause of a lack of organized convection?
Rainamount(mm d-1)Rain rate [mm d-1]
Latit
ude
BCC−CSM1.1
−60−30
0
3060
BNU−ESM CCSM4 CESM1−BGC
CMCC−CESM
−60−30
0
3060
CMCC−CMS CNRM−CM5 CSIRO−Mk3−6−0
CanESM2
−60−30
0
3060
FGOALS−g2 GFDL−CM3 GFDL−ESM2G
GFDL−ESM2M
−60−30
0
3060
INM−CM4 IPSL−CM5A−LR IPSL−CM5B−LR
MIROC−ESM
−60−30
0
3060
MIROC−ESM−CHEM
1 10 100
MIROC5
1 10 100
MPI−ESM−LR
1 10 1001 10 100
Rain distributions:Models & Observations
SANDY
24 OCTOBER2012
40mm d-1
Tracking individual storms (upper: Sandy, lower:Irene) using TempestExtremes to find storm centersfrom ERA5 pressure. Compare tracks with the EPIC-ORCA tracked 95th percentile IMERGE rainfall.
High-impact events
IRENE
24 AUGUST2011