Verification Overview

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Presentation transcript:

Verification Overview (based on CP activity: JJA2016-MAM2017) Alexander Kirsanov & WG5 Verification Overview, COSMO GM, 11-14 Sept 2017, Jerusalem

VERIFICATION OVER THE COMMON AREA COSMO-7, COSMO-EU, COSMO-GR, COSMO-I7, ICON-EU, IFS, ICON, COSMO-ME, COSMO-PL, COSMO-RU7 Annual reports and Seasonal analytics are located at the website: http://cosmo-model.org/content/tasks/verification.priv/

General Information on Scores Continuous parameters Performance Diagram Temperature at 2 m Dew point temperature at 2 m Pressure reduced to Mean Sea Level Wind speed at 10 m Total cloud cover Dichotomic parameters Total Precipitation in 6 hours Total Precipitation in 24 hours Extremal Dependence Indices

00 UTC Run and 12 UTC Run score difference is not significant 00 UTC Run and 12 UTC Run score difference is not significant, except some scores of 2m Dew Point Temperature and a few precipitation scores.

TEMPERATURE AT 2M From: 2016-06-01 To: 2017-05-31 ME Diurnal variability underestimation: negative ME during day, positive ME during night RMSE ICON-EU/ICON: the lowest RMSE and diurnal score variations Last year tendency: JJA RMSE ↓ SON RMSE ↓ DJF RMSE ↑ MAM RMSE ↑

DEW POINT TEMPERATURE AT 2M From: 2016-06-01 To: 2017-05-31 ME ICON-EU/ICON positive ME is decreasing with lead time: Spinup effect? ICON (and ICON-EU) ME is decreasing with lead time especially during JJA and SON, 00 UTC Run RMSE ME and RMSE maximum is during the late daytime Last year tendency: JJA RMSE ↓ DJF RMSE ↑ MAM RMSE ↑

TOTAL CLOUD COVER From: 2016-06-01 To: 2017-05-31 ME COSMO → ME>0 ICON-EU/ICON → ME~0 IFS → ME<0 RMSE ME and RMSE maximum during nighttime Last year tendency: ME and RMSE decrease for most COSMO models

WIND SPEED AT 10 M From: 2016-06-01 To: 2017-05-31 ME ICON-EU/ICON has closest to zero ME, less notable diurnal ME variation Last year tendency: SON RMSE ↓ ME is decreasing

Precipitation in 6h 0.2 mm threshold From: 2016-06-01 To: 2016-08-31 The most significant diurnal variation and the lowest (worst) Threat Score compared to other seasons ICON, ICON-EU, and IFS overestimate low precipitation more than COSMO models: Presumably, The IFS/ICON cumulus convection scheme is responsible? Low precipitation overestimated, strongest overestimation during daytime

Precipitation in 6h 0.2 mm threshold From: 2016-12-01 To: 2016-02-28 Low precipitation overestimated Threat Score is better than during summer Less than during other seasons diurnal variation and differences between models Scores can be divided into warm season (JJA and MAM) and cold season (DJF and SON) groups with similar patterns

Precipitation in 6h 0.2 mm threshold From: 2017-03-01 To: 2017-05-31 IFS overestimates low precipitation more than ICON-EU/ICON during MAM-2017 and SON-2016 IFS overestimates low precipitation more than ICON during MAM and SON yet the Threat Score is higher for IFS in case of SON (not shown)

Precipitation in 24h 10 mm threshold From: 2017-03-01 To: 2017-05-31 High precipitation events are underestimated ICON-EU/ICON underestimate high precipitation events the least

Precipitation in 6h JJA-2016: EDI EDI&SEDI show diurnal variability with minimum values during 12-18 UTC for JJA and MAM, during 18-24 UTC for DJF and SON Precipitation in 6h DJF-2017: EDI EDI&SEDI values are decreasing for higher precipitation events, decreasing with the lead time Precipitation in 24h JJA-2016: EDI

VERIFICATION OVER THE COMMON AREA 2: FINE RESOLUTION COSMO-1, COSMO-DE, IFS, ICON, COSMO-IT, COSMO-PL

Dew point temperature at 2 m scores are slightly better for High resolution models, compared to coarse resolution models, especially for COSMO-1 and COSMO-PL Coarse Res. High Res. T2M, PMSL, TCC , WSPD Fine Resolution Domain scores are not significantly better than the scores of Coarse resolution models

Precipitation in 6h 0.2 mm threshold From: 2017-03-01 To: 2017-05-31 Common Area 2: Fine Resolution Common Area: Coarse Resolution Added value of high resolution: COSMO-1 shows the best scores Generally, there are better scores for High Resolution models (than for Coarse Resolution models) for low precipitation events…

Precipitation in 24h 10 mm threshold From: 2016-12-01 To: 2017-02-28 Common Area 2: Fine Resolution Common Area: Coarse Resolution …but for high precipitation events and longer accumulation period High Resolution models are not significantly better

CONCLUSIONS 00 UTC Run and 12 UTS Run score difference is not significant (good news!) ICON scores are close to IFS scores and are notably better for T2m, Td2m, and for a number of precipitation scores (!!!) ICON, ICON-EU, and IFS overestimate low precipitation more than COSMO models: presumably, The IFS/ICON cumulus convection scheme is responsible? COSMO show less overestimation of low precipitation events compared to IFS, ICON, and ICON-EU, the most significant in this regard is added value of High Resolution COSMO versions ICON, ICON-EU and IFS have the mean error around zero or negative, while the COSMO versions mainly overestimate total clouds Overestimation of 10 m wind speed decreased for most models during the last three years, and the RMSE improved

Thank you for your attention

PRESSURE REDUCED TO MEAN SEA LEVEL From: 2016-06-01 To: 2017-05-31 RMSE RMSE minimum during nighttime for warm seasons JJA and MAM Last year tendency: JJA RMSE ↓ SON RMSE ↓ DJF RMSE ↓ MAM RMSE ↓

LONG TREND PRECIPITATION with high resolution stations LOW THRESHOLDS Very slightly positive/steady trend seasonal oscillation LAM perform better than ECMWF (low thres.) ETS for run00 for each model Seasonal trend starting from djf04 till mam17 First and second day Very low threshold 2 mm in 24 h Comments: Slightly positive trend General better performance for LAM Long-term trends of COSMO models performance over Italian catchment areas, Elena Oberto, Naima Vela, Flora Gofa

LONG TREND PRECIPITATION with high resolution stations HIGH THRESHOLDS Very slightly positive trend Big seasonal oscillation ECMWF often performs better than LAM (medium-high thres.) ETS for run00 for each model Seasonal trend starting from djf04 till mam17 First and second day High threshold 20 mm in 24 h Comments: Slightly positive trend Light better performance for IFS with respect LAM Long-term trends of COSMO models performance over Italian catchment areas, Elena Oberto, Naima Vela, Flora Gofa

LONG TREND PRECIPITATION with high resolution stations LOW THRESHOLDS Ecmwf overestimation Summer overestimation Reduction of the overestimation for LAM BIAS for run00 for each model Seasonal trend starting from djf04 till mam17 First and second day Very low threshold 2 mm in 24 h Comments: Systematic overestimation for IFS General summer overstimation General bias reduction for LAMs during last year Long-term trends of COSMO models performance over Italian catchment areas, Elena Oberto, Naima Vela, Flora Gofa

LONG TREND PRECIPITATION with high resolution stations HIGH THRESHOLDS General underestimation, especially 7, IFS Seasonal cycle Worse the second day BIAS for run00 for each model Seasonal trend starting from djf04 till mam17 First and second day High threshold 20 mm in 24 h Comments: Pronounced seasonal error cycle General underestimation for IFS, 7 ecc.. General bias increasing during the second day Long-term trends of COSMO models performance over Italian catchment areas, Elena Oberto, Naima Vela, Flora Gofa