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Activities of WG7 Chiara Marsigli.

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Presentation on theme: "Activities of WG7 Chiara Marsigli."— Presentation transcript:

1 Activities of WG7 Chiara Marsigli

2 Task 1 - Development of COSMO-LEPS
Maintenance and updates of the operational suite at ECMWF Revision of the clustering and member selection techniques started Calibrated COSMO-LEPS 24h precipitation forecasts calibrated QPF are operationally generated (for subdomains) Addition of multi-model driven members COSMO-HYBEPS suite running from 7th September 2012 Tests for the LAM-EPS BC project with COSMO-LEPS activity coordinated within SRNWP ET-EPS, cases selection on-going

3 Task 2 - Development of an ensemble system for the Sochi Olympic Games
COSMO-FROST-EPS running and providing data to HMC part of CORSO PP

4 Task 3 – Perturbation of the surface fields
Development of soil moisture perturbations Stopped due to lack of resources

5 Task 4 - Verification of ensemble forecasts
Collaboration with WG5 and VERSUS for ensemble forecasting verification tools for EPS verification are being implemented in VERSUS, support provided by WG7 for score definition (parallel session this afternoon)

6 Task 5 - Development of convection-permitting ensembles
Product development and evaluation at MCH Verification of COSMO-LEPS, evaluation of COSMO-DE-EPS Study towards a COSMO ensemble at 2.8 km over Italy First tests on parameter and LBC perturbations Tests for the LAM-EPS BC project to drive convection-permitting EPS Coordinated within SRNWP ET-EPS EPS will be run at T1279 for two 2-week periods, providing BCs for testing the impact on existing LAM-EPSs and higher resolution downscaling Periods selection is on-going

7 Development of convection permitting ensembles
during last WG7 meeting (March 2012) it was decided to prepare a document providing a framework for coordinating convection-permitting ensemble in COSMO A draft has been circulated within WG7 and will be finalised during this meeting. It addresses: Future of COSMO-LEPS Feasibility of a COSMO implementation at higher resolution Plans of the COSMO members Highlight common interests Identify possibilities for cooperation (new PP on ensemble?)

8 KENDA/WG7 meeting A common interest is the use of KENDA to provide IC perturbations to the ensembles -> need to enforce the link with KENDA KENDA/WG7 meeting yesterday afternoon: how to best proceed to ensure good coordination between DA and EPS developments? discussion is continuing tonight!

9 FINE


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