Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss First COSMO-E experiments with SPPT COSMO General Meeting.

Slides:



Advertisements
Similar presentations
Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss Improving COSMO-LEPS forecasts of extreme events with.
Advertisements

Ensemble activities in COSMO C. Marsigli, A. Montani, T. Paccagnella ARPA-SIM - HydroMeteorological Service of Emilia-Romagna, Bologna, Italy.
WG7 summary and Science Plan Chiara Marsigli ARPA Emilia-Romagna, SIMC.
Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss WG5-Report from Switzerland: Verification of COSMO in.
Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss Quantitative precipitation forecasts in the Alps – first.
Ensemble Post-Processing and it’s Potential Benefits for the Operational Forecaster Michael Erickson and Brian A. Colle School of Marine and Atmospheric.
Institute of Meteorology and Water Management – NRI Extensive tests of lower-boundary-variation-based COSMO EPS COTEKINO Priority Project -
COSMO General Meeting Zurich, 2005 Institute of Meteorology and Water Management Warsaw, Poland- 1 - Verification of the LM at IMGW Katarzyna Starosta,
Francesca Marcucci, Lucio Torrisi with the contribution of Valeria Montesarchio, ISMAR-CNR CNMCA, National Meteorological Center,Italy First experiments.
Performance of the MOGREPS Regional Ensemble
Ensemble-variational sea ice data assimilation Anna Shlyaeva, Mark Buehner, Alain Caya, Data Assimilation and Satellite Meteorology Research Jean-Francois.
SLEPS First Results from SLEPS A. Walser, M. Arpagaus, C. Appenzeller, J. Quiby MeteoSwiss.
ESA DA Projects Progress Meeting 2University of Reading Advanced Data Assimilation Methods WP2.1 Perform (ensemble) experiments to quantify model errors.
COTEKINO Priority Project COSMO WG7 Chiara Marsigli.
Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss Parametrization of Subgrid-Scale Orographic Drag in the.
Eidgenössisches Departement des Innern EDI Bundesamt für Meteorologie und Klimatologie MeteoSchweiz Statistical Characteristics of High- Resolution COSMO.
WWOSC 2014, Aug 16 – 21, Montreal 1 Impact of initial ensemble perturbations provided by convective-scale ensemble data assimilation in the COSMO-DE model.
ISDA 2014, Feb 24 – 28, Munich 1 Impact of ensemble perturbations provided by convective-scale ensemble data assimilation in the COSMO-DE model Florian.
Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss Task 1 of PP Interpretation 1.1Further applications of.
SEASONAL COMMON PLOT SCORES A DRIANO R ASPANTI P ERFORMANCE DIAGRAM BY M.S T ESINI Sibiu - Cosmo General Meeting 2-5 September 2013.
COSMO General Meeting, Offenbach, 7 – 11 Sept Dependance of bias on initial time of forecasts 1 WG1 Overview
Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss Conditional verification of all COSMO countries: first.
Latest results in verification over Poland Katarzyna Starosta, Joanna Linkowska Institute of Meteorology and Water Management, Warsaw 9th COSMO General.
Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss Accounting for Change: Local wind forecasts from the high-
Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss Cost Efficient Use of COSMO-LEPS Reforecasts Felix Fundel,
Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss Verification results of COSMO at MeteoSwiss in the year.
Sensitivity experiments with the Runge Kutta time integration scheme Lucio TORRISI CNMCA – Pratica di Mare (Rome)
Operational ALADIN forecast in Croatian Meteorological and Hydrological Service 26th EWGLAM & 11th SRNWP meetings 4th - 7th October 2004,Oslo, Norway Zoran.
HNMS contribution to CONSENS Petroula Louka & Flora Gofa Hellenic National Meteorological Service
. Outline  Evaluation of different model-error schemes in the WRF mesoscale ensemble: stochastic, multi-physics and combinations thereof  Where is.
Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss Local Probabilistic Weather Predictions for Switzerland.
Eidgenössisches Departement des Innern EDI Bundesamt für Meteorologie und Klimatologie MeteoSchweiz First Experience with KENDA at MeteoSwiss Daniel Leuenberger,
Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss Quantitative precipitation forecast in the Alps Verification.
Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss WG 4 activities.
Verification Verification with SYNOP, TEMP, and GPS data P. Kaufmann, M. Arpagaus, MeteoSwiss P. Emiliani., E. Veccia., A. Galliani., UGM U. Pflüger, DWD.
10 th COSMO General Meeting, Krakow, September 2008 Recent work on pressure bias problem Lucio TORRISI Italian Met. Service CNMCA – Pratica di Mare.
Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss WG 3: Overview status report COSMO General Meeting, 19.
Deutscher Wetterdienst Fuzzy and standard verification for COSMO-EU and COSMO-DE Ulrich Damrath (with contributions by Ulrich Pflüger) COSMO GM Rome 2011.
Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss Science Plan, PPs, PTs, and more … COSMO General Meeting,
Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss Status of the COSMO-1 configuration at MeteoSwiss Guy.
Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss A more reliable COSMO-LEPS F. Fundel, A. Walser, M. A.
General Meeting Moscow, 6-10 September 2010 High-Resolution verification for Temperature ( in northern Italy) Maria Stefania Tesini COSMO General Meeting.
Deutscher Wetterdienst Preliminary evaluation and verification of the pre-operational COSMO-DE Ensemble Prediction System Susanne Theis Christoph Gebhardt,
Overview of WG5 activities and Conditional Verification Project Adriano Raspanti - WG5 Bucharest, September 2006.
Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss Component testing of the COSMO model’s turbulent diffusion.
PP CONSENS Merging COSMO-LEPS and COSMO- SREPS for the short-range Chiara Marsigli, Tiziana Paccagnella, Andrea Montani ARPA-SIMC, Bologna, Italy.
VERIFICATION Highligths by WG5. 2 Outlook Some focus on Temperature with common plots and Conditional Verification Some Fuzzy verification Long trends.
A study on the spread/error relationship of the COSMO-LEPS ensemble Purpose of the work  The spread-error spatial relationship is good, especially after.
Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss Status of the COSMO-1 configuration at MeteoSwiss Guy.
Setting up COSMO EPS perturbing lower boundary conditions Riccardo Bonanno, Nicola Loglisci COSMO General Meeting - Eretria – 8-11 September 2014 COTEKINO.
Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss Experiments at MeteoSwiss : TERRA / aerosols Flake Jean-Marie.
ALADIN 3DVAR at the Hungarian Meteorological Service 1 _____________________________________________________________________________________ 27th EWGLAM.
OSEs with HIRLAM and HARMONIE for EUCOS Nils Gustafsson, SMHI Sigurdur Thorsteinsson, IMO John de Vries, KNMI Roger Randriamampianina, met.no.
Eidgenössisches Departement des Innern EDI Bundesamt für Meteorologie und Klimatologie MeteoSchweiz Ensemble activites and plans at MeteoSwiss André Walser.
Wrap-up of SPPT Tests & Introduction to iSPPT
Studies with COSMO-DE on basic aspects in the convective scale:
Nigel Roberts Met Reading
André Walser MeteoSwiss, Zurich
Tuning the horizontal diffusion in the COSMO model
WG5-Report from Switzerland: Verification of aLMo in the year 2005
COSMO General Meeting 2009 WG5 Parallel Session 7 September 2009
Observation uncertainty in verification
A. Topographic radiation correction in COSMO: gridscale or subgridscale? B. COSMO-2: convection resolving or convection inhibiting model? Matteo Buzzi.
Thomas Gastaldo, Virginia Poli, Chiara Marsigli
Verification of COSMO-LEPS and coupling with a hydrologic model
Preliminary test for the development of a 2.8km ensemble over Italy
Christoph Gebhardt, Zied Ben Bouallègue, Michael Buchhold
Some Verification Highlights and Issues in Precipitation Verification
Short Range Ensemble Prediction System Verification over Greece
Activities of WG7 Chiara Marsigli.
Presentation transcript:

Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss First COSMO-E experiments with SPPT COSMO General Meeting 2 September 2013, Sibiu André Walser, Daliah Maurer, Marco Arpagaus

COSMO-1: 8x daily O(24 hour) forecasts 1.1km grid size (convection permitting) Boundary conditions: IFS 10km 4x daily Project COSMO-NExT COSMO-E: 2x daily 5 day forecasts 2.2km grid size (convection permitting) O(21) ensemble members Boundary conditions: VarEPS 20km 2x daily ensemble data assimilation: LETKF

COSMO-E setup Ensemble forecasts with convection-permitting resolution (2.2 km mesh-size) 21 members Twice a day up to +120h for Alpine area (15% larger than COSMO-2 domain) Range of possible scenarios and “best estimate” COSMO version 4.26 Single precision, reduction of elapsed time to 60% with same forecast quality!  talk in POMPA session Tue afternoon

COSMO-NExT (and related) talks Mon 09:10 (WG1/WG7): First COSMO-E experiments with SPPT Mon 10:20 (WG4): Status of COSMO-1 development at MeteoSwiss Mon 11:00 (WG5): Verification of the experimental version of COSMO-1: Winter-Spring 2013 Mon 11:30 (WG3a): Turb-i-Sim: Evaluation and improvement of COSMO turbulence over Alpine topography Mon 12:00 (WG1): First Experience with KENDA at MeteoSwiss Tue 14:55: EXTPAR developments towards version 2.0

Outline COSMO-E physics perturbations: Validation of stochastic perturbation of physics tendencies (SPPT) scheme Impact of SPPT settings based on case studies Results from a 2 weeks test suite COSMO-E LBCs First results from BC-EPS experiments Outlook

G. J. Shutts, ECMWF

Implementation into COSMO by L. Torrisi (CNMCA)

Validation of SPPT SPPT must not degrade quality of members  show-stopper deterministic runs for different SPPT setups: for all: lgauss_rn = lhorint_rn = ltimeint_rn =.true. ex0: no SPPT ex1: SPPT, recommended settings by Lucio (sigma = 0.25 & random number within [-0.75, 0.75]) ex2: lqv_pertlim =.true. ex3: sigma = 0.5 & random number within [-1.0, 1.0] ex4: length-scale = 0.5 deg., time-scale = 30 min (default: 5 deg., 6 hrs) ex5: no tapering in lower troposphere / PBL (default: tapering below approx. 850 hPa)

Upper-air verification all stations: Payerne, Milano, München, Udine, Stuttgart, Kümmersbruck, Wien, Praha, Zagreb, Nimes, San Pietro temperature, rel. humidity, wind speed and direction, geopotential +72h lead time

Upper-air: temperature +72h, all stations,

Upper-air: wind speed +72h, all stations,

Upper-air: wind direction +72h, all stations,

Upper-air verification: conclusions largest differences found for wind speed and direction in summer: ex3 shows larger STDE minor negative impact for ex1 minor positive impact for ex4 marginal differences between all experiments for T, Z, and RH  no drying observed!

Surface verification scores vs lead-time ~ 500 stations following slides show the largest differences between experiments

Surface: dew-point temperature all stations, bias standard deviation drying in ex3

16 COSMO-E: stochastic physics | objective verification Daliah Maurer, Marco Arpagaus, and André Walser Surface: wind speed all stations, bias standard deviation ex3 shows largest bias and standard deviation

17 COSMO-E: stochastic physics | objective verification Daliah Maurer, Marco Arpagaus, and André Walser Surface: precipitation, 12h sum all stations, bias frequency bias (10mm) For summer precipitation ex3 belongs to the best experiments…

18 COSMO-E: stochastic physics | objective verification Daliah Maurer, Marco Arpagaus, and André Walser Surface: precipitation, 12h sum all stations, bias frequency bias (10mm) …but for winter precipitation ex3 it is the worst one

Surface verification: conclusions small differences between all experiments, except for ex3 which shows larger STDE for some parameters drying in summer (Td_2m) higher precipitation amounts (worse in winter, better in summer)  No significant quality degradation seen with SPPT except for ex3 (largest random numbers together with large correlation-lengths)

COSMO-E SPPT case studies Experiments for 2 summer and 2 autum cases investigated SPPT perturbations only (no IC and BC pert.) COSMO-2 domain (instead of new COSMO-E domain) ICs: COSMO-2 analysis LBCs: IFS-ENS control

No tapering in lower troposphere Main motivation to taper SPPT in PBL are stability issues SPPT validation runs did not show any Turn it off has significant impact on spread in PBL -- off -- on 250m above ground 700m above ground tropopause Temperature spread over Swiss domain

Impact of SPPT settings on spread large stdv_rn=0.5, range_rn=1 (ex3) stdv_rn=0.25, range_rn=0.75 (ex1) stdv_rn=0.25, range_rn=0.75, dlat_rn=dlon_rn=0.5°, ninc_rn=90 (ex4) Case : T spread COSMO-E domain spread largest at 850 hPa, lowest at 500 hPa spread saturation is reached at all height levels at about same lead-time larger random numbers produce larger spread and faster spread growth smaller correlation-lengths in space and time lead to smaller 500 (solid lines), 700 (dashed), 850 (dotted) hPa

Impact of SPPT settings on spread Case : T spread ~250 m above ground +72h small sigma/range large space/time correlation large sigma/range small space/time correlation

First COSMO-E test suite 2 weeks period ( – ) 00 UTC forecast only Experiments with 3 setups: LBC + SPPT: lqv_pertlim=.false. (default=.true.) dlat_rn=dlon_rn=0.5 (5.0) ninc_rn=180 (1080) stdv_rn=0.5 (0.5) range_rn=1.0 (1.0) no tapering near surface (code change) setup validated as well (not show before) LBC + COSMO-DE-EPS parameter perturbation (PP) LBC only scale of convective systems

Comparison of ensemble dispersion Normalized Variance Difference (NVD, Clark et al. 2009) Range = [-1,+1] LBC+SPPT vs. LBC, precipitation > 1mm/12h LBC+SPPT show larger ensemble dispersion but difference decreases with increasing lead-time

Verification COSMO-E test suite focus on lead-times beyond 24 hours due to lack of IC perturbations unfortunately VERSUS not yet ready at MCH for EPS first step: against COSMO-2 analysis (ad-hoc)

Rank histogram LBC+SPPT +24h +72h +120h temperature ~5500m above ground too small spread up to +72h but too large spread for end of forecast range

Spread & error temperature mean squared error mean ensemble variance ~5500m ~700m LBC+SPPT too small spread in boundary layer too large spread for end of forecast range

Spread & error temperature mean squared error mean ensemble variance ~5500m ~700m LBC+SPPT LBC+PP LBC LBC+SPPT LBC+PP LBC LBC+PP and LBC slightly smaller spread LBC show largest error LBC+SPPT best, but differences small

Spread & error wind speed mean squared error mean ensemble variance ~5500m ~700m LBC+SPPT LBC+PP LBC LBC+SPPT LBC+PP LBC Too small spread in PBL for wind speed as well LBC+SPPT rather too large spread in upper troposphere

Reliability diagram LBC-SPPT +48h +96h high reliability in particular for longer lead-times good resolution even for longer lead-times precipitation > 5mm/12h

Verification COSMO-E test suite focus on lead-times beyond 24 hours due to lack of IC perturbations unfortunately VERSUS not yet ready at MCH for EPS first step: against COSMO-2 analysis (ad-hoc) second step: against SYNOP observations (movero)

Brier Skill Score (ref=climatology) Reference: forecast based on station climatology (300 stations) better worse than clim. forecast all experiments clearly better than clim. forecast for all lead-times LBC+SPPT best until +72h, but differences very small

Brier Skill Score (ref=climatology) better worse than clim. forecast Reference: Forecast based on station climatology (300 stations) daytime precip. only slightly better than clim. forecast LBC+SPPT best experiment

Brier Score decomposition All experiments very similar: very good reliability resolution only slightly decreasing with increasing lead-times reliability (the lower the better) resolution (the higher the better) BS (the lower the better) based on 500 stations

Conclusions COSMO-E experiments Surprisingly large reduction in spread with smaller correlation lengths for random numbers SPPT produces only small additional spread for runs with LBC perturbations 3 setups LBC+SPPT, LBC+PP and LBC show similar results but impact of SPPT larger than of PP spread in PBL clearly too small in PBL… …but rather too large in upper-air with LBC+SPPT only slightly better scores with SPPT so far experiments shows surprisingly high reliability for precipitation probabilities (enough statistics?)

Representing uncertainty initial conditionsboundary conditionsmodel physics Implementation of perturbations KENDA

BC-EPS experiments ECMWF provide 2 BC-EPS data sets for 3 periods: current resolution T L 639 (~32 km)  BCR high resolution T L 1279 (~16 km)  BCH winter storm period – run with COSMO-E (without SPPT) first results show slightly better scores with BCH in surface verification (500 stations)

Brier score 12h sum of precipitation BCH shows better scores mainly thanks to better resolution

Brier Score 10m wind gusts BCH slightly better strangely, brier score gets better with increasing lead-time…

Outlook continue work with SPPT (internship of Daliah Maurer) extend test suite (more statistics) analyse characteristics of SPPT term in model equations try to generate more spread near-surface without increasing upper-air spread including IC perturbation from KENDA implementation of SKEB in COSMO with Judith Berner (COSMO activity proposal) detailed analysis of BC-EPS experiments and perform runs for other 2 periods