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COSMO Steering Committee Meeting 21-22 March 2019 , Offenbach a. M., Germany

COSMO Steering Committee Meeting 21-22 March 2019 , Offenbach a. M., Germany. SPM Slides ( dmiitrii.mironov@dwd.de). To highlight some points.

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COSMO Steering Committee Meeting 21-22 March 2019 , Offenbach a. M., Germany

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  1. COSMO Steering Committee Meeting 21-22 March 2019, Offenbach a. M., Germany SPM Slides (dmiitrii.mironov@dwd.de) COSMO STC Meeting, 21-22 March 2019, Offenbach a. M., Germany

  2. To highlight some points • SMC>> indicates issues on which decision was taken at one of the previous SMC meetings (particularly at the SMC meeting in Offenbach in February 2019) • STC>>indicates issues that call for the STC decision/feedback

  3. 6. COSMO-LEPS (20 min) • 6.1. ECMWF computer resources • 6.2. Future development • During 2019 • Migration from 7 km to 5 km horizontal mesh size (5kmL45) • Use of new COSMO-model version 5.06 • STC>> STC approval is required (increase in BUs)

  4. COSMO-LEPS : proposed upgrade In May, November andDecember 2018, thefollowingexperimentshavebeenperformed: runsof 20-member COSMO-LEPS at 5 km, 45 ML, 10-members Tiedtke + 10-members Bechtold, version 5.05 in SP: results still tobefullyanalysed (bug 5.05 in SP?) During 2019, thefollowingactivityisproposed: migrationtoresolutions5km/45ML (now 7km/40ML) (-> subjectto STC approval), laggedensembleusing also ENS from 18UTC and 06UTC, COSMO vers. 5.03 in SP migrationto COSMO version 5.06 SMC>> SMC discussion in February: Improvementfrom 7 to 5 km not so clear (shownfor May, but with a multi-physicsensemble), possibleconsiderationof different upgrades (e.g. numberofmembers) NOTE: latestbythe end of 2019 andbetterbeforethan August 2019 (due to ECMWF HPC moving), weshouldusesoftware (COSMO, int2lm, fieldextra, ...) running on ecCodes, asgrib_api will bedismissed

  5. RPSS: tp06h ROC: tp06h May 2018 experimentation: oper7vs test5 • RPSS: clear daily cycle in the performance of the model; higher skill of test5 in the short range for day-time precipitation; mixed results later on. • ROC area: slight positive impact of enhanced resolution for all thresholds.

  6. t2m wspeed10m May 2018 experimentation: oper7vs test5 • T2M: some reduction of rmse at night-time for test5; larger spread for oper7 (effect of perturbed parameters, missing in test5 so far) • WSPEED10M: no impact on spread by enhanced resolution; slight systematic reduction of rmse of the ensemble mean.

  7. COSMO-LEPS upgrade: 2) is an alternative proposal 5km Horiz/45lev in thevertical (usingCOSMO SP, same as OPER) + laggedensembleusingalso ENS from 18UTC and 06UTC Parallel disseminationcanstart in June 2019, migrationcanstart in Nov2019 About 3 timesmore expensive in SBU than OPER SPPT + Multiphysics+ COSMO DP + laggedensembleusing also ENS from 18UTC and 06UTC migrationcanstart in June 2019 Onlyabout1.5 timesmore expensive in SBU than OPER (due tothe double precision)

  8. COSMO-LEPS upgrade - tests SPPT (test on JJ2015 and NDJ2014-2015, COSMOv5.01) Improvementspreadandskillfor TP (especially large thresholds) and T2m Multiphysics(10 members Tiedtke + 10 membersBetcholds) + COSMOv5.04 (test on AM2017) Improvementskillfor TP (all thresholds) Multiphysics+ 5km Horiz/45lev Vertresolution + COSMOv5.05 SP (test on M2018 and D2018) Improvementspreadandskillfor TP (all thresholdsandespecially at thefirst time ranges) andimprovementofskillforT2m and Wspeed10m, detrimentforspread T2m 1) 3) 2)

  9. In experiment 3) in ordertoseeonlythecontribution of theresolutionincrement, wecomparedtheperformance of thetwoensemblesub-sets of 10members usingonly Tiedtkescheme Variable: 6h cumulatedprecipitation (thresholds: 1, 5, 10, 15, 25, 50 mm). May 2018. Scores: RankedProbability Score (RPS), ROC area at fixedfc. range, ROC area at fixedthreshold ROC area: positive impact of enhancedresolution at all TimeRanges, alwaysforthresholds > 5mm andespeciallyfor high ones. RPS: slighthigherskillfornoonprecipitation Relative impactoftheresolutionincrement

  10. 7.1. WG1, KENDA-O • Christoph Schraff PP KENDA-O (Christoph Schraff) • Runs until: Aug 2020 • Info at COSMO web: OK • FTEs: no FTEs for Dec 2018 - Feb 2019

  11. Status Report for KENDA-O (+ WG1) • Task 1: further development of LETKF scheme (conventional obs) •  MCH: Claire Merker (2-y) on developing regional static B matrix: • (progress slowed down due to search for a bug & reduced resources) •  differences in impact of DA components (e.g. radar radial winds, • additive covariance inflation) on COSMO-D2 and COSMO-DE found, • which need to be understood better and are being investigated further •  preliminary implication: conclusions from C-DE experiments cannot be • translated to C-D2 readily !! (or to other model configurations) • Task 2: extended use of obs: ongoing work, mostly progressing ok, but: • negative impact of radar radial winds in DWD parallel suite for autumn / C-D2 • radar Vr removed from parallel suite again • recently: found bug (data assimilated twice  experiment with bug fix started) • and data quality issues (mainly at night / autumn + spring) found • Task 3: soil moisture analysis using satellite SM data: fellowship ends ~ now! • (no clear benefit yet, will continue tests in parallel suite, with little (!) FTE) • (however, this is not critical for the whole KENDA project)

  12. Status Report for KENDA-O (+ WG1) • Task 4: adaptation to ICON-LAM: progressing well despite some (non-critical) delays: •  MEC-based ILAM-LETKF without SST- / Snow Analysis already clearly better • than COSMO-LETKF in most parameters • (for 2-week summer period, C-DE, w/o LHN which requires further tuning) • first tests with ICON-D2 mostly ok (better than C-DE in some var., worse in upper-air wind) • first tests with SST-/ Snow Analysis included in DA cycle started • implementing capability of calling DACE observation operators in ICON • for full 4-D online LETKF for ICON-LAM in early summer • pre-operational suite ICON-LAM with LETKF from autumn 2019 • towards EnVar (3DVar): • COSMO-DE test: (MEC-based) 3-D LETKF not much worse than (online)4-D LETKF •  not detrimental when losing 4-D capability with (3-D) EnVar • (even 4-D EnVar feasible in longer term) •  EnVar potentially promising (Var approach has algorithmic advantages) • preliminary version of MEC-based 3DVAR + EnVar exists • May / June: COSMO obs operators in DACE + TL/Adjoint (required for Var) • later on: testing (regional B-matrix from MeteoSwiss project needed!), • final aim: pure LETKF replaced by hybrid LETKF/EnVar (for EPS/determ.)

  13. Supplementary info on KENDA-O Task 2: use of additional obs Note: ‘O’ stands for ‘for the use of High-Resolution Obs’ Decision on obs types for which work is (about to be) fully focused on ICON-LAM thus abandoning the aim to introduce them operationally with COSMO (at DWD) and thus within the time frame of PP KENDA-O • Radar Radial Winds yes if possible, but depends on results • Radar Reflectivity ICON (operational introduction possibly together with ICON-LAM) • (but ARPAE: radar reflectivity foreseen pre-operational by end of 2019 • required: regular reception of volumes from Nat Dept. Civil Protect) • GPS ZTD / STD pursued further for COSMO • SEVIRI WV (clear-/all-sky)  ICON • SEVIRI VIS (WG1) ICON • Lightning (WG1) ICON • Screen-level (T2m,q2m…) open (next steps with COSMO) • Mode-S already operational • other data (e.g. ground-based remote sensing (lidar etc.)): DWD currently not active •  not in COSMO at DWD (but maybe at other centres?) Minor issues will be continued to be developed for COSMO-model in the near future(e.g. on modified / new BUFR templates, redundancy check, processing of tower data, radiosonde descent data, high-resolution radiosonde data, quality control, bug fixes, etc.)

  14. 7.2. WG2, CDIC*, CELO*, EX-CELO, CCE • Michael Baldauf

  15. 7.2. WG2 (cont’d) • PP CDIC (Michael Baldauf) • PP completed in Aug 2018 • Final report pending • FTE tables OK(please check info at COSMO web, incl. the FTE tables) • PT CELO (Bogdan Rosa) • PP completed in Aug 2018 • Final report pending • "Project resources" summary at the top of PP page is missing (see other PPs as examples) • FTE tables OK

  16. 7.2. WG2 (cont’d) PP EX-CELO (Zbigniew Piotrowski) • Runs until: Sep 2019 • Info at COSMO web: OK (but please update “Project resources” at the top of PP page, incl. PP duration, FTEs used, etc.) • FTEs: no FTE entries • Note: PP implementation delayed, no significant progress since GM 2018; extension will be requested • PT CCE (Damian Wojcik) • Runs until: Sep 2019 • Info at COSMO web: OK (PT plan of 07.08.2018 is available) • FTEs: no FTEs for Dec 2018 - Feb 2019

  17. Status WG2 March 2019 M. Baldauf, withhelpfrom D. Wojcik, B. Rosa, G. Zängl M. Baldauf (DWD)

  18. PP CELO (COSMO-EULAG operationalization) • Sept. 2012 - Aug 2018, finished • COSMO-EULAG runspre-operational at IMGW since June 2018 • PP final/technicalreportisunderpreparation (consultationswith P. Smolarkiewicznecessary) • PP EX-CELO (Extension of COSMO-EULAG operationalization) • Sept. 2017 - Aug. 2019 • onlyfewworksince GM (due toGridTools implementations …). Coupling of EULAG to COSMO 5.05 is a bit of double work with PP CCE due to different code base by GridTools-version • unplanned: coworker (Farnoush) left the project in August • current plans: get COSMO 5.05 running with one-to-one correspondence with the C++ implementation. M. Baldauf (DWD)

  19. PP CCE (Consolidationof COSMO-EULAG) • Sept. 2018 - Aug. 2019: new • 1. Migratingtoandverificationof COSMO-EULAG 5.5 • 2. MPDATA for TKE-Advection • 3. Climatesimulationswith COSMO-EULAG (coll. with BTU Cottbus) • Implementation of the domain decomposition independent calculations; the restart is ready; and the CE is supplemented with the zero-gradient b.c. option for precipitating variables. • Implementation of TKE advection with MPDATA is done. • update of the Scientific Documentation of the model with the help of P. Smolarkiewicz’ review. • PP CDIC (Comparisonofdynamicalcoresof ICON and COSMO) • Sept. 2015 – Aug. 2018, finished • Straka et al. (1993) testcaseis still not ready • PP final = technicalreportisoverdue (prob. not before May 2019, i.e. after ‚PDEs on thesphere‘) M. Baldauf (DWD)

  20. Short-term plans • for COSMO model: • Higher order scheme (Univ. Cottbus) was planned for COSMO 5.6.Unfortunately, A. Will was not available for several months, therefore, the work stopped. Hopefully, we can deliver this for COSMO 5.7… • No further work for COSMO (RK)! • for ICON-LAM(after discussionwith G. Zängl) • Investigation ofdiffusion/dampingpropertiesofthe ICON-dyn. core • divergencedampingshouldn‘tbenecessaryforthedyn. corealone; however, itisneededfordiffusion on the large time step • Physics-dynamicscoupling • example: precipitationspectraof ICON-LAM and COSMO seemtobequite different. Why? •  possible PT? M. Baldauf (DWD)

  21. Medium- tolong-term plans Higher orderdiscretizationbased on DiscontinuousGalerkinmethods (mass-, momentum-, energy-conserving, …) example: Straka et al. (1993) testcase DG 3rd ordertoymodelwith dx=200m! Reference solutionwith dx=25m (fromStraka et al., 1993) However, a lotofinvestigationsnecessarybefore an implementationinto ICON isreasonable… M. Baldauf (DWD)

  22. 7.2. WG2 (cont’d) • SMC>> Extensive discussion at the February 2019 SMC meeting (OF) of the future contribution (beyond September 2019) of EULAG team to the ICON-LAM (based on the outcome of the September 2018 SMC meeting (SPb) and on the suggestions by Andrzej Wyszogrodzki) [further discussion at WG2 meeting during ICCARUS 2019] • Implementation of the EULAG dynamical core into ICON does not seem to be reasonable since the ICON dynamical core already fulfils the properties of mass- and tracer-mass conservation, overall 2nd order convergence, and satisfactory treatment of steep terrain • If comparison of COSMO-EULAG and ICON is to be made, its outcome must be clearly defined • Further suggestions • Investigation of diffusion and damping properties of the ICON core • Tests of ICON (physics) at very high resolution and a comparison between ICON at high and at very high resolution (sub-km, CLM interest, Uni Cottbus)

  23. 7.3. WG3a, ConSAT*, T2(RC)2 • Matthias Raschendorfer (see February 4, 2019, summary) • SMC>> • Work has been slowed down due to Matthias’ health condition, the situation improves now

  24. 7.3. WG3a (cont’d) PT ConSAT(Matthias Raschendorfer) • Runs until: PT completed (note that ConSATwas neither considered nor approved by the STC in 2017, so formally it did not exist as PT) • No information at the COSMO web, no FTE table entries; would be good to provide some information, e.g. a brief summary of the work performed

  25. 7.3. WG3a (cont’d) PP T2(RC)2 Phase 2 (Harel Muskatel) • Runs until: Aug 2019 • Info at COSMO web: OK • FTEs: no FTEs for Dec 2018 - Feb 2019

  26. PP T2(RC)2: final steps • Current state: • Still running and expected to be ready at the end of current COSMO year: • implementation and the testing of CAMS prognostic aerosols => ICCARUS talk by Harel M. • Investigation the effect on 2-moment microphysics with heterogeneous ice-nucleation • investigating the effect of the Segal & Kahinscheme for water-droplet nucleation • on rain production and radiation transfer => ICCARUS talk by Harel M. • Implementation of all new features for cloud-radiation coupling in official COSMO-version • Finalized as a matter of prototypic development: • Derivation of optical cloud properties from shallow convection (SC) =>last-year talk by Pavel K. • Direct calculation of optical properties in a convective plume model based on adiabatic lifting => JAS article by Pavel K. et al. • Positive test results of the developed components for COSMO • A remaining issue: • Consistent combination of sub-grid cloud processes with contributions from parameterized turbulence and convection • Future planning: A new 2-year PP as a follower with focus on ICON • Possibly related to the use of prognostic aerosols or a consistent parametr. of sub-grid cloud processes • Not more than an idea so far; needs to be discussed after consultation of the main agents

  27. Ad ConSAT: as an action of WG tasks • Related to Radiation: • An inconsistency with regard to the vertical distribution of aerosol mass from 2D aerosol climatology was detected and corrected in ICON (affecting clear-sky radiation and thus the surface heat budget): • Avoids a certain loss of aerosol mass correlated with the height of mean topography • Is not an issue for Tanre, but is possibly for Tegen, Kinne or CAMS in COSMO! • Related to TURBDIFF and TURBTRAN: • ICON config. (being available in COSMO as well) with (old) COSMO config. of TERRA in parallel test-suite at DWD • Clear improvements of T_2m and Td_2m; reduction of nocturnal BIASes • Some not yet understood problems have to be tackled for ensemble runs • Reformulation of current “circulation term” in TKE scheme into a “thermal SSO term” • Describes the action of sub-grid ana- and kata-batic winds rather than thermal surface patterns • Is dependent on SSO parameters • First implementation in private developing branch of ICON seems to work • Supplements in TURBTRAN • Enabling an implicit dependency of transfer velocities on surface temperature • Fully implemented, is going to be released together with associated TERRA revision • Final testing could not be completed due to illness

  28. Ad ConSAT: as an action of WG tasks • Related to TERRA in ICON (including some interfaces): • Major reorganization of the code with an as far as possible implicit treatment of surface temperature • Additional heat budget for snow-free surface skin • Implicit solution for linearly coupled heat budgets for fractional snow cover, snow-free surface skin and subjacent soil • Lots of inconsistencies being incompatible with an implicit treatment had to be removed: • Rewrite of dynamic snow-tile aggregation and the TERRA interface • Extensive adaptations of old and recently introduced intricate workarounds in TERRA • Removes the drastic time-step oscillations of (near-)surface temperatures at large time steps • Already allows the specification of a skin resistance between uppermost soil layer and surface • Is a prerequisite and proper preparation of the full cover-layer implementation (canopy) • Fully implemented in priv. dev. branch; final testing could not yet be completed due to illness • Prototype of (snow-free) cover-layer exists as test-version of former COSMO-TERRA and will be used for the full cover-layer implementation in ICON-TERRA (under consideration of snow) • Planning the implementation of a new Multi-Layer (ML) snow-model (<-> PT SAINT): • Snow heat budget formulated as a ML extension in rewritten test version of ICON-TERRA • All the ML snow hydrology is encapsulated in a subroutine, providing TERRA with variables necessary for solving the heat budget and using updated T_snow profiles from TERRA

  29. 7.4. WG3b, CALMO-MAX, TERRA Nova, AEVUS, SAINT • Jean-Marie Bettems

  30. 7.4. WG3b(cont’d) PP CALMO-MAX (Antigoni Voudouri) • Runs until: Aug 2019 (extension requested, being considered by SMC) • Info at COSMO web: OK (further information at the WG3b page) • FTEs: no FTEs for Dec 2018 - Feb 2019 • PT TERRA Nova (Yiftach Ziv) • Runs until: Feb 2019 (completed) • Final report expected in June 2019 • Info at COSMO web: OK (PT plan of 08.08.2018 is available, further information at the WG3b page) • FTEs: OK

  31. 7.4. WG3b(cont’d) PT AEVUS (Paola Mercogliano) • Runs until: Jun 2019 • Info at COSMO web: OK (further information at the WG3b page) • FTEs: no FTE entries for many 3-month periods (please check/provide with due regard for delays) PT SAINT (Sascha Bellaire) • Runs until: June 2020 • Info at COSMO web: OK (PT plan of 13.10.2017 of is available, further information at the WG3b page, incl. Annex A of January 2019) • FTEs: no FTEs for Sep 2018 - Feb 2019

  32. PP CALMO-MAX, 06.2017 – 09.2019 • Automatic calibration is a very important tool for the community • differenttargetdomainwithdifferentclimatology… • different model configuration… • development of new parameterization… • CALMO methodologyisrecognized as a relevant approach • 2 publishedpapers in refereedpapers (Atm. Research) • regularlyusedat ETHZ for climaterun calibration • willbeapplied at B-TU (calibration COSMO with new dycoreby A.Will) • model independentmethod

  33. PP CALMO-MAX, 06.2017 – 09.2019 • Status • Meta-model refinementsimplemented ( GitHub) • COSMO-1 calibration done, impact beinganalyzed • Technical infrastructure beingprepared at ECMWF • Discussion on standard procedure for documentation of unconfined model parametershas started • Open questions • Definitive proof of the benefit for NWP (target area withdifferentclimatologythan Central Europe) • How to achieve an acceptable cost for the method(in particularwhen the soil memory issignificant)? • How to handleweatherdependency of the optimal parametersvalues?

  34. PP CALMO-MAX, 06.2017 – 09.2019 • The PL asks for a one year PP extension (09.2019 09.2019);resources at HNMS and IMS are secured (1.8 FTEs);thisissupported by the WG3bC • A one year extension is mainly required to fulfill CALMO-MAX goals associated with the optimization of the methodology and the definition of a standard procedure on model parameter documentation. • Based on the knowledge, available at HNMS and at IMS a permanent support for CALMO based calibration for the COSMO community could also be envisaged.

  35. PT SAINT, 07.2017 – 06.2020 • Multi-layers snow model, essentially based on SNOWPACK (SLF / Davos) • Offers a very good base for any sort of future developments (e.g. effect of deposited aerosols on snow albedo) • 1 yearextensionfunded ( 06.2020) • Agreement with Matthias R. on theimplementation, waitingforinterfacecode • First completeversionplannedforMid-April 2019 (in a private COSMO coderelease) • Visit at DWD planned around end April to coordinate transfer of development in an official COSMO release, and in an official ICON-LAM release • Standaloneversioncouldbequiteuseful (analysis, climate…) and will beevaluated • Code ownertobedefined (couldbe Juergen Helmert) SMC>> Need to co-ordinate Sascha’s and Matthias’ efforts and to have the code owner is stressed (progress is already made in terms of co-ordination, Jürgen tentatively agrees)

  36. PT AEVUS, 09.2017 – 06.2019 • Bulk urban parameterizationby Hendrik W., skintemperatureforvegetationby Jan-Peter S. • Promissingresults (UHI, circulation), but quite a lotoftechnicalissueswiththecode • Workshop at Torino 12/2018, Offenbach 03/2019, Ghent 04/2019 (with Hendrik) • Candidatefor COSMO v6.0 • Follow-upenvisaged : focus on ICON-LAM & externalparameters

  37. PT TERRA Nova, 09.2016 – 02.2019 • Tests of multiple modelconfigurations on different targetareas • Large delay due tolateavailabilityof COSMO v5.05, and due totechnicalproblemswiththemoreadvanced TERRA configurations • Comparison with Community Land Model (MSc Verena B.) points towards the missing vegetation layer being one main deficiency of TERRA • Workshop at ICCARUS 2019, final report will bepreparedafterwards

  38. 7.5. WG4, CORSO-A* • Anastasia Bundel • PP CORSO-A (Gdaly Rivin, Inna Rozinkina) • PP completed • Final report is ready and will appear at the COSMO web shortly

  39. WG4 Current activities • Collection of cases of model failures (~2-4 cases from each member) is ongoing, results to be presented during the GM • CORSO-A final report is ready for publication at the COSMO site • New WG5-WG4 PP AWARE “Appraisal of challenging weather forecasts”. The goal is to provide the COSMO community with an overview of forecast methods and forecast evaluation approaches linked to high impact weather (HIW) (more details in Flora’s presentation) • as before: most active in the group: MCH, IMGW-PIB, HNMS, RHM; lack of commitment from some members

  40. 7.6. WG5, INSPECT*, CARMA • Flora Gofa

  41. 7.6. WG5 (cont’d) • PP INSPECT (Flora Gofa, Anastasia Bundel) • PP completed in Dec 2017 • Final report is available at COSMO web • Info at COSMO web, incl. the FTE tables, OK PP CARMA (Amalia Iriza-Burca) • Runs until: Mar 2020 • Info at COSMO web: OK (but please update “Project resources” at the top of PP page) • FTEs: FTE tables prepared (new project), no FTEs for Dec 2018 - Feb 2019

  42. PP INSPECT Anastasia Bundel (1), Flora Gofa (2) (PP leaders) and Dmitry Alferov (1), Elena Astakhova (1), Petra Baumann (4), Dimitra Boukouvala (2),, Ulrich Damrath (3), Pierre Eckert (4), Alexander Kirsanov (1), Xavier Lapillonne (4), Joanna Linkowska (5), Chiara Marsigli (6), Andrea Montani (6), Anatoly Muraviev (1), Elena Oberto (7), Maria Stefania Tesini (6), Naima Vela (7), Andrzej Wyszogrodzki (5), and Mikhail Zaichenko (1), André Walser (4) • Final Technical report available on COSMO web • http://www.cosmo-model.org/content/model/documentation/techReports/docs/techReport37.pdf • Collaboration with MesoVICT international community is continuing. MesoVICT final meeting was announced during the recent monthly webconf (January ‘19). Necessity for a few WG5 people to participate if resources are available. • List of publications extracted from MesoVICT and possibly a final paper summarizing the main outcomes of MesoVICT • PP-INSPECT work to be continued partially by PP-AWARE (Task4)

  43. Common Plot Activity 2018-2019 • Guidelines prepared by WG5c and sent in Oct (WG5 web repository) • Web page content with Annual Report for 2017-2018 (available on web, HNMS) • and Seasonal Common Plots for JJA-SON 2018 (available, RHM) • Keep the standard parameter scores for CM1 and CM2 to maintain long term • trends • Continue analysis with Wind Performance Rose for wind sp/dir (ArpaE) • Include FSS plot analysis (Arpa-PT) • PROCEDURE • Input data adaptation (LIBSIM) • FSS calculation for period 10-11/2018 (VAST) for 1-2 forecastdays • Calculation of percentage of FSSuseful for eachcombination of precipitationintensity/spatial • GRIDS/MODELS • 0.03°: COSMO IT, COSMO 2I, COSMO D2, COSMO 1(?) • 0.04°: COSMO PL (limited area) • 0.07°: COSMO I5, COSMO GR. • OBSERVATION • Opera database (retrieved and processed in grib format by HNMS) • STC>> Requestfor additonalFTEs for FSS (0.075FTEs?) COSMO SMC meeting, 5-6 February 2019

  44. PP CARMA • Task 1. First Level Support Implementation and Training Start 12.2018 – End 04.2019 – ON-GOING • 1.1 Documentation review (MEC-Rfdbk), analysis of new material required. • Start 12.2018 – End 01.2019 - completed • 1.2 Documentation preparation for CP activity content (MEC-Rfdbk) • Start 01.2019 – End 02.2019 - on-going • 1.3 Preparation of a complete example set of data (one season, one model) to be used • Start 01.2019 – End 02.2019 –completed • 1.4 Training provided by DWD experts for first level support to the PST (Project Support Team) • Start 03.2019 – End 03.2019 • Slight delay due to scheduling conflicts;will take place between 09-11 April 2019 • 1.5 Implementation of the MEC-Rfdbk system @NMA and @HNMS (PST). • Start 03.2019 – End 05.2019 • 1.6 Adaptation of scripts for the production of the CP requirements (Task 1.2) • Start 05.2019 – End 06.2019 • 1.7 Setup of web interface with the use of Shiny R routines on COSMO server • Start 05.2019 – End 06.2019 • Task 2. Second Level Implementation and support Start 05.2019 – End 10.2019 • Contributors:PST and NMSs responsible person • Task 3. Cross-validation of implementation Start 09.2019 – End 12.2019 • Contributors: PST and NMSs responsible person • Task 4. Implementation of CP activity content Start 10.2019 – End 12.2019 • Contributors: PST and NMSs responsible person • Task 5 Elaboration of guidelines for CARMA (MEC-Rfdbk) system use Start 12.2019 – End 02.2020 • Contributors: A. Iriza-Burca (NMA), F. Gofa (HNMS) • Estimated resources (in FTE-years) needed in total: 3.450 FTEs (mostly in 2019)

  45. 7.7. WG6, CEL-ACCEL, POMPA*, IMPACT, SPRT • Massimo Milelli

  46. 7.7. WG6 (cont’d) • PP POMPA (Xavier Lapillonne) • PP completed in Jul 2018 • Final report pending • Info at COSMO web, incl. the FTE tables, OK • PP CEL-ACCEL (Zbigniew Piotrowski) • See WG6 slides 6-7 (link) • Runs until: Sep 2019 • Info at COSMO web: OK (but please update “Project resources” at the top of PP page, incl. PP duration, FTEs used, etc.) • FTEs: no FTEs for Sep 2018 – Feb 2019 • Note: PP implementation delayed, extension for 6 (12) months will be requested

  47. 7.7. WG6 (cont’d) • PP IMPACT (Carlos Osuna) • Runs until: Sep 2022 • Info at COSMO web: OK (but please update “Project resources” at the top of PP page) • FTEs: FTE tables prepared (new project), no FTEs for Sep 2018 - Feb 2019 • PP WG6-SPRT (Massimo Milelli) • Runs until: permanent • Info at COSMO web: OK • FTEs: OK

  48. 7.8. WG7, SPRED*, CIAO*, APSU • Chiara Marsigli

  49. 7.8. WG7 (cont’d) • PP SPRED (Chiara Marsigli) • PP completed in Feb 2018 • Final report ready (should soon appear at COSMO web) • Info at COSMO web, incl. the FTE tables, OK (but please checkthe FTE tables and FTE summary) • PT CIAO (Andrea Montani) • PT completed in Dec 2018 • Would be good to get a brief summary of results • FTEs: no FTEs for Sep 2018 - Feb 2019

  50. 7.8. WG7 (cont’d) • PP APSU (Chiara Marsigli) • Runs until: Aug 2020 • Info at COSMO web: OK • FTEs: no FTEs for Dec 2018 - Feb 2019

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