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Data assimilation in Aladin. Claude Fischer; Thibaut Montmerle; Ludovic Auger; Lo ï k Berre; Gergely Boloni; Zahra Sahlaoui; Simona Stefanescu; Arome collaborators. Data assimilation inside Aladin. 3 « operating Centers »: Budapest, Toulouse (operational), Casablanca (run daily) - PowerPoint PPT Presentation
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September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in Aladin
Data assimilation in AladinData assimilation in Aladin
Claude Fischer; Thibaut Montmerle; Ludovic Auger; Loïk Berre;
Gergely Boloni; Zahra Sahlaoui; Simona Stefanescu;Arome collaborators
September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in Aladin
Data assimilation inside AladinData assimilation inside Aladin
• 3 « operating Centers »: Budapest, Toulouse (operational), Casablanca (run daily)
• Dispatched research collaborations: Bratislava (radar), Brussels (wavelet), Bucarest (ensembles, methods), Lisbon (ensembles), Ljubljana (nudging), Prague, Tunis (surface analysis), Sofia (surface analysis and snow), Zagreb (methods)
• Existing tools: – Optimal Interpolation (« CANARI ») both for 3D and surface, – 3D-VAR (screening and minimisation), – TL and adjoint Eulerian hydrostatic models
September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in Aladin
Variational system: what is in it ?Variational system: what is in it ?
• Incremental 3D-VAR, using 80-90 % of the common Arpège/IFS code
• Continuous assimilation cycle, 6 hour frequency, long cut-off assimilation cycle and short cut-off production, coupled with Arpège, Analysis=Model gridmesh=9.5km
• Observations:– Surface pressure, SHIP winds, synop T2m and RH2m– Aircraft data– SATOB motion winds– Drifting buoys– Soundings (TEMP, PILOT)– Satellite radiances: AMSU-A, AMSU-B, HIRS, Meteosat-8 SEVIRI– No QuikSCAT
• Digital filter initialisation
September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in Aladin
Ensemble B matrixEnsemble B matrix
• Bi-periodic spectral structure functions (a torus)• Control variable: vorticity + unbalanced divergence, (T, Ps)
and specific humidity• Background error covariances are sampled from an
ensemble of Aladin forecasts, with initial conditions from an ensemble of Arpège analyses: « ensemble Jb »
• Sample: over 48 days, two pairs of 6 hour forecasts are extracted from the ensemble, and their difference is computed => 96 elements in the sample
• For the time being, constant uniform σb
bxxx
xbxHyRTxbxHyxBTxxJ
)H)((1)H)((1)(2
September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in Aladin
Data processing :• 1 pixel out of 5 is extracted and thinning boxes of 70 km are applied• IR 3.9 and 13.4 as well as ozone 9.7 are blacklisted, as well as IR channels over land• predictor, situation-dependent bias correction applied to the other channels• empirical o are used• first-guess quality control removes too large innovations• CMS/Lannion cloud classification is used to keep IR 8.7 10.8 ,12 only in clear sky while the two WV channels are also kept over low clouds
Use of Météosat-8/SEVIRI in the 3DVar of Use of Météosat-8/SEVIRI in the 3DVar of ALADINALADIN
Cloud types
Vertical weighting functions
September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in AladinDyn. Adapt. Raingauges
3DVar 3DVar with SEVIRI
Impact study :Precipitation forecast
2004/07/18 12UTCRR P12 – P6
September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in Aladin
Operational implementation in Aladin-FranceOperational implementation in Aladin-France
• A one month period over June 2003• A two week period in July 2004• First E-suite: March 23rd through May 22nd, 2005• Second E-suite: June 2nd through July 25th, 2005
=> operations started on Monday, July 25th
September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in Aladin
About scores: About scores: 3D-VAR3D-VAR versus versus Dyn. Adapt.Dyn. Adapt.
Mean sea level pressure 3 hour cumulated
precipitations2m relative humidity
bias
RMS
September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in Aladin
Scores w/r to radiosondesScores w/r to radiosondes
Temperature biasTemperature RMS
Wind biasWind RMS
Blue: 3D-VAR > Dyn Adapt
Red: 3D-VAR < Dyn Adapt
September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in AladinA specific case: June 21st, 2005
September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in Aladin
June 21st: Aladin modelJune 21st: Aladin modelP12-P6 RR
3D-VAR
September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in Aladin
June 21st: Aladin model (.)June 21st: Aladin model (.)P18-P12 RR
3D-VAR
September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in Aladin
E-suites: V1 and V2E-suites: V1 and V2• V1: 23 March through 22 May, 2005 =>
– Deteriorated MSLP bias and RMS by about 0.2 hPa– Too strong precipitation amounts at short range (6h, 12h), with significant spin-down– Analyses too wet compared to RS– No increase in the number of « Aladinades » (which is a relief, given the problems on
humidity and RR)• V2: started 2nd of June, scheduled for about 1.5 month
– Improved SEVIRI bias correction, using a case/location-dependent b.c. (with 4 predictors)
– Infrared channels over land blacklisted (problem of poor quality surface temperature)– Additional surface observations ready: T2m, RH2m => quite complementary with
SEVIRI data– Digital filter initialization: back to settings from dynamical adaptation– Reduced weighting of Jo with respect to Jb: Sb decreased from 3.24 to 2.25
September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in Aladin
Lessons from Aladin-France:Lessons from Aladin-France:• Precipitations:
– [0,3h] => caution (impact of initialisation, of imbalances …); – [3,12h] => the assimilation cycle(s) produce their own solution; – [12,24h] => a limit of predictability somewhere in this range, mostly
due to the growing influence of lateral boundary conditions; – RMS(Dyn Adap – 3DVAR) for 6 hour precipitation (mm/6h), for three
days of the test period:
07/07 08/07 22/07
P12-P6 2.32 2.08 1.75
P24-P18 1.37 1.44 1.10
September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in Aladin
3DVAR at the Hungarian Met Service3DVAR at the Hungarian Met ServiceShort history:• Implementation with French and Slovak help (June 2000)• November 2002: Quasi-operational parallel suite• Operational application (May 2005)
Basic characteristics:
• 6h 3DVAR assim. cycle
• 48h production
• linear grid
• dx ~ 8km
• 49 vertical levels
September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in Aladin
3DVAR at the Hungarian Met Service3DVAR at the Hungarian Met Service
Assimilation details:
• 6h cycle (4 long + 2 short cut-off analyses per day)
• ARPEGE fields for surface
• local 3DVAR for upper air
• NMC background error statistics
• DFI initialization
• 3h coupling in cycle (by the long cut-off ARPEGE analyses and the corresponding 3h forecasts)
Input observations:
• SYNOP: surface pressure
• TEMP: temperature, wind, pressure, specific humidity
• ATOVS/AMSU-A radiances
• AMDAR aircraft reports: temperature, wind
All the observation types above are used in the ARPEGE assimilation system too, but in a somewhat worse resolution!
September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in Aladin
3DVAR at the Hungarian Met Service3DVAR at the Hungarian Met Service
Objective scores:
• generally small improvement for temperature and wind
• neutral impact/improvement on high level’s geopotential
• degradation in low level’s geopotential and MSLP BIAS
• mixed impact on humidity
Subjective evaluation:
• improvement in T2m (0-24h)
• improvement in precipitation (0-48h)
• degradation (0-24h) / neutral impact (24-48h) in cloudiness
• neutral impact on wind
Assimilation results vs the spin-up version
September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in Aladin
September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in Aladin
In the near future, for Aladin-FranceIn the near future, for Aladin-France• 3D-VAR FGAT• Jk extra cost function to fit towards the ARPEGE analysis• Test 3-hourly analyses• Better understand the intrication between digital filter
initialization, coupling and B-matrix dynamical balances• Innovating observations for the mesoscale: sampling of
satellite data, QuikSCAT• Application for AMMA
• Code convergence with the Hirlam group: mesoscale multi-incremental 4D-VAR and an increasing collaboration on very high resolution (Arome-oriented 2.5 km)
• Next 4 year mid-term Aladin scientific plan
mid-term issues, for the collaboration:mid-term issues, for the collaboration:
September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in Aladin
4-year mid-term scientific plan: Aladin (with 4-year mid-term scientific plan: Aladin (with Arome input)Arome input)
• Variational assimilation:– « B »: wavelets, ensemble sampling, non-linear and Ω-equation,
gridpoint σb and cycling, humidity control variable– Algorithms: 3D-VAR FGAT, 4D-VAR in a nutshell– Observations: satellite (cloudy IR, microwave, locally received
data, impact of bias correction, wind retrievals), GPS zenital delay, radar reflectivity and Doppler winds, 2m and 10m mesonet
• Surface analysis:– Ocean and sea ice SAF SST derived from geostationnary
satellites– Snow analysis (with Hirlam), possibly using land SAF snow
cover– Off-line soil analysis using « dynamical OI »
• Diagnostic fine-grid 3D-VAR hourly analysis for nowcasting
September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in Aladin
Thank you for your attentionThank you for your attention
September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in Aladin
End of talkEnd of talk
Now come some extra slides for whatever …
September 19-23 , 2005 23COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in Aladin
Tuning of background and observation error Tuning of background and observation error variancesvariances
• Desroziers and Ivanov, 2001:(So, Sb) ?
– For a consistent systemSo = Sb = 1
• For a LAM system: – How to compute the Trace ? -> Monte-
Carlo method (Girard, 1987)– How to compute the statistical
expectation ? -> use a time mean over a suitably long range
– Samples of small size -> aggregate analysis times together
– Applied to the NMC statistics
)()(2)(
)()(2)(
min
,
min
,
KHTrJES
HKITrJES
bSSb
p
oSSo
bo
bo
Sadiki and Fischer, Tellus, 2005
Chapnik etal., QJRMS, 2004
September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in Aladin
Sensitivity experimentsSensitivity experiments
3d-Var ALADIN experiments over 1
month
NMC-laggedbackground=P06H
0.86 < 1 1.67 > 1
Standard NMC statistics
0.6 0.53
Ensemble statistics --- 1.44 (by comparison with NMC)
oS bS
18.0 oS 3d-Var ARPEGE
September 19-23 , 2005COSMO D.A. Workshop and 7th COSMO General Meeting
Data assimilation in AladinStatistics in the space of observationsStatistics in the space of observations
ARPEGE4D-VAR
ALADIN3D-VAR
radiosondes
ATOVS channels