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A.Montani; The COSMO-LEPS system.
Recent developments and plans for the
COSMO-LEPS system
Andrea Montani,
C. Marsigli, T. Paccagnella
ARPA-SIMC
HydroMeteoClimate Regional Service of Emilia-Romagna, Bologna,
Italy
COSMO General meetingLugano, 10-13 September 2012
A.Montani; The COSMO-LEPS system.
Outline
• Recent upgrades of COSMO-LEPS: implementation of 00UTC COSMO-LEPS, modifications in the set-up of members’ perturbations, implementation of calibrated precipitation.
• Performance of the system: time-series verification of COSMO-LEPS using SYNOP, case study assessment (“nevone 2012”).
• Present/future work:modifications to the clustering/selection technique,first tests of COSMO-HYBrid-EPS.
• Summary and plans
A.Montani; The COSMO-LEPS system.
Main changes during the COSMO year (1)
• 30 November 2011, COSMO-LEPS “doubles”:
• a new ECMWF time-critical application was prepared and sent to ECMWF as for the implementation of COSMO-LEPS also at 00UTC (cleps00);
• cleps00 and cleps12 have identical configurations (use of COSMO-EU analysis fields also for cleps00 since 18 January 2012);
• cleps00 is potentially more exposed to product delays because of ECMWF system sessions (never happened so far).
• 29 March 2012, no more random choice of the convection scheme:
• following requests of DWD, members 1-8 use Tiedtke convection scheme, members 9-16 use Kain-Fritsch.
• 3 July 2012, system upgrades:
• COSMO model upgraded to 4.21 + perturbation tuning;
• generation of calibrated 24-h TP over Germany, Switzerland, Emilia-Romagna;
• archive of ECMWF-EPS model level fields at 0.25x0.25 on a large domain to enable reruns (last 3 months).
A.Montani; The COSMO-LEPS system.
COSMO-LEPS suite @ ECMWF: present status
d-1d-1 dd d+5d+5d+1d+1 d+2d+2 d+4d+4d+3d+3
older EPSolder EPS
younger EPSyounger EPS
clustering clustering periodperiod
0000
1212
Cluster Analysis and RM identificationCluster Analysis and RM identification
4 variables4 variables
Z U V QZ U V Q
3 levels3 levels
500 700 850 hPa500 700 850 hPa
2 2 time time stepssteps
Cluster Analysis and RM identificationCluster Analysis and RM identification
European European areaarea
Complete Complete LinkageLinkage
16 Representative Members driving the 16
COSMO-model integrations (weighted according to the cluster
populations)
using either Tiedtke or Kain-Fritsch convection scheme (members 1-8 T,
members 9-16 KF) +
perturbations in turbulence scheme and
in physical parameterisations
COSMO-LEPS
clustering area
• suite runs twice a day (00 and 12UTC) as a “time-critical application” managed by ARPA-SIMC;
• Δx ~ 7 km; 40 ML; fc+132h;• COSM0 v4.21 since July 2012;• computer time (30 million
BUs for 2012) provided by the ECMWF member states in COSMO.
COSMO-LEPS
Integration Domain
A.Montani; The COSMO-LEPS system.
Outline
• Performance of the system: time-series verification of COSMO-LEPS using SYNOP; case study assessment (“nevone 2012”).
A.Montani; The COSMO-LEPS system.
– SYNOP on the GTS
Time-series verification of COSMO-LEPS
Main features:
variable: 12h cumulated precip (18-06, 06-18
UTC);
period : from Dec 2002 to Jul 2012;
region: 43-50N, 2-18E (MAP D-PHASEPHASE
area);
method: nearest grid point; no-weighted fcst;
obs: synop reports (about 470
stations/day);
fcst ranges: 6-18h, 18-30h, …, 102-114h, 114-126h;
thresholds: 1, 5, 10, 15, 25, 50 mm/12h;
system: COSMO-LEPS;
scores: ROC area, BSS, RPSS, Outliers, …
both monthly and seasonal scores were computed
A.Montani; The COSMO-LEPS system.
Time series of ROC area Area under the curve in the HIT rate vs FAR diagram; the higher, the better … Valuable forecast systems have ROC area values > 0.6.
Highest scores in the second part of 2011 for all but the highest threshold.
fc 30-42h: ROC area is low for the highest threshold for last winter; then recovery.
fc 78-90h: in the last months, some recovery of the score for the 15mm threshold, after a “difficult” beginning of the year.
Limited loss of predictability with increasing forecast range.
A.Montani; The COSMO-LEPS system.
Heavy snowfalls in Emilia-Romagna (31/1 – 5/2/2012)
A.Montani; The COSMO-LEPS system.
COSMO-I7 of 30/01/2012 12UTC (+36-60h)+36-60h
Snow observed (cm) over the 24-hour period ending at 00UTC of 2/2/2012
forecasts (mm of equivalent water!)
A.Montani; The COSMO-LEPS system.
COSMO-LEPS of 30/01/2012 12UTC (+36-60h)
available at 23.30 UTC
A.Montani; The COSMO-LEPS system.
COSMO-LEPS of 30/01/2012 12UTC (+36-60h)
COSMO-LEPS forecasts give early indication of possible heavy snowfall over the plain.COSMO-LEPS signal remained more stable and consistent than COSMO-I7.
A.Montani; The COSMO-LEPS system.
Outline
• Present/future work:modifications to the clustering/selection technique,first tests of COSMO-HYBEPS.
A.Montani; The COSMO-LEPS system.
Test modifications of clustering methodology
• Consider distances between ECMWF EPS members according to “COSMO-LEPS metric” (Z, U, V, Q in the mid-lower troposphere over the clustering domain).
• Look at distances between pairs of ECMWF EPS members; to what extent do these distances grow with forecast range (in “COSMO-LEPS metric”)?
• Study a number of seasons.
Outcome: modifications to the number of clusters / number of global EPSs considered / clustering intervals.
A.Montani; The COSMO-LEPS system.
COSMO-HYBrid Ensemble Prediction System
From the results of CONSENS PP, come to a synthesis with the different ensemble systems / strategies, considering scientific, implementation, solidity aspects.
Generate 20-member hybrid ensemble (COSMO-HYBrid-EPS), where:
a) 16 members comes from COSMO-LEPS,
b) 1 member is nested on IFS (with Tiedtke scheme),
c) 1 member is nested on IFS (with Kain-Fritsch scheme),
d) 1 member is nested on GME,
e) 1 member is nested on GFS.already existing from CONSENS.
All members have Δx ~ 7 km; 40 ML; fc+132h.
Study performance of different members’ combinations with the same ensemble size.
“20-members esuite” implemented on 7/9/2012;
will be run up to the end of the year.
A.Montani; The COSMO-LEPS system.
Main results
Time-series verification:ECMWF EPS changed substantially in the last years (more and more weight to EDA-
based perturbations) and it is hard to disentangle improvements related to COSMO-
LEPS upgrades from those due to better boundaries; nevertheless:– highest values of BSS and ROC area for the probabilistic prediction of 12-h precipitation
for autumn 2011;
– poor performance in the first months of 2012, then recovery. Need to investigate what
happened.
Case-study verification:consistent signal of high-impact weather events for the snowfalls of February 2012.
Other achievements:• provision of ICs and BCs for convective-permitting ensembles;
• operational dissemination implemented for Romania;
• reorganisation of post-processing with Fieldextra.
A.Montani; The COSMO-LEPS system.
• Test modifications to the clustering methodology.
• Test COSMO-HYBrid-EPS.• Increase vertical resolution? ensemble size? ... tonight’s discussion.
• LAMEPS_BC project consider possible modifications to COSMO-LEPS suite.
• COSMO-LEPS for TIGGE-LAM (GRIB2 encoding).
• COSMO-LEPS twice a day: generate probabilistic products from lagged ensembles.
Future plans
• Support calibration and verification ( Versus?).
• Carry on collaboration within research project (HyMeX, EFAS, SAFEWIND,
IMPRINTS, …).
A.Montani; The COSMO-LEPS system.
Thank you !