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HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service CNMCA – Pratica di Mare (Rome) [email protected]

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Page 1: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

Precipitation Computed by COSMO-ME model (PR ASS1)

Lucio TORRISI

Italian Met. Service CNMCA – Pratica di Mare (Rome)

[email protected]

Page 2: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

Overview• PR ASS1 products

– Description– Generation– Use

• Precipitation computed by a NWP model

• Objective Verification• Future developments

Page 3: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

PR ASS1 products• The purpose of the computed precipitation

products is to support other H-SAF products, e.g. by providing first guess fields or filling occasional gaps in the operational chains for satellite product generation.

• PR-ASS1 (Quantitative Precipitation Forecast) products are available at fixed times of the day: 00, 03, 06, 09, 12, 15, 18 and 21 UTC.

• These products consists of: – accumulated precipitation (AP) over 3, 6, 12 and 24

hours preceding the nominal time;– precipitation rate (PR) at nominal time.

Page 4: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

Precipitation rate

Maps are in equal latitude/longitude projection. Data in GRIB format

Page 5: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

Accumulated precipitation

Maps are in equal latitude/longitude projection. Data in GRIB format

Page 6: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

PR ASS1 Operational Suite

The WP-2200 activity is embedded in the development of the operational NWP system of CNMCA.

Satellite observations

End-users and H-SAF central archive

COSMO-ME model integration

Ground-based and aircraft observations

Accumulated precipitation Precipitation rate

Data assimilation (3DVar)

Page 7: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

14 km

7 km

2.8 km

- hydrostatic equations- parameterized convection

- compressible equations- parameterized convection

- compressible equations- explicit convection

CNMCA NWP System

Data Assimilation

72h

24h

Page 8: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

PR ASS1 GenerationPR ASS1 products are generated as forecasts (PR/AP) or forecast differences (AP) from the most appropriate COSMO-ME model run preceding the nominal time (currently two runs a day 00-12 UTC). At 00 UTC:

D 00 UTCD-1 00 UTC D-1 12 UTC

D-1 00 + 24h

D-1 12 + 12h

D-1 12 + 12h minusD-1 12 + 6h

D-1 12 + 12h minusD-1 12 + 9h

D-1 12 + 12hPR

AP 3

AP 6

AP 12

AP 24

+12 h

+9 h

+6 h

+12 h

+12 h

+12 h

+24 h0 h

0 h

Page 9: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

File name conventions

URL: ftp://ftp.meteoam.it username: hsafpassword: 00Hsaf

directory: products

Product identifier: h06.Folders under h06:

h06_yyyymm_grb archived data of previous monthsh06_yyyymm_png

h06_cur_mon_grbdata of current month

h06_cur_mon_png

Files description:h06_yyyymmdd_hh_ii_rom.grb digital data

h06_yyyymmdd_hh_ii_rom.png image data

yyyymm: year, month

yyyymmdd: year, month, day

hh: nominal synoptic hour to which the product refers (00, 03, 06, 09, 12, 15, 18, 21 UTC)

ii: integration interval (00, i.e. instantaneous precipitation, and previous 03, 06, 12 or 24 hours)

Page 10: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

How to use the GRIB file

• A decoding programme (C language) for COSMO-ME GRIB files (provide geographical coordinates and values at each grid point) is available in the ftp site as the products, in:

• To run the programme:– install grib_api library

(http://www.ecmwf.int/products/data/software/download/grib_api.html)

– change the GRIB_API_INSTDIR in the Makefile according to your grib api installation directory;

– launch make; – use the executable file generated as follows:

grib1_decode.ex <grib file>

ftp://[email protected]/utilities/grib1_decode/

Page 11: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

COSMO-ME uses a rotated lat-lon grid. To derive the geographical coordinates from the rotated ones:

COSMO-ME Horizontal Grid

where

North pole

Page 12: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

Precipitation Computed by a NWP Model

• Precipitation forecast fields computed by a NWP model will be used in HSAF to provide spatio-temporal continuity to the observed fields, otherwise affected by temporal and spatial gaps due to insufficient and inhomogeneous satellite cover.

• “Computed” precipitation by a model is partitioned into two fractions: – the grid-scale precipitation: it refers to the production

of precipitation, via atmospheric processes that may be resolved in a NWP model, such as areas where upward motion will ultimately lead to clouds and precipitation (also referred to as explicit condensation)

– the parameterized (or convective) precipitation: which is devised to capture the sub-grid scale cumulus convection (by-product of cumulus parameterization schemes)

• The partitioning into the components depends on the mesh size

Page 13: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

Grid-Scale Clouds/Precipitation Param.

• The primary interest in the numerical modelling of grid-scale clouds and precipitation (water-continuity model) is the behaviour of the overall ensemble of particles.

• In COSMO model (www.cosmo-model.org) a fully prognostic one-moment bulk water-continuity scheme including five water categories is used (vapour, water, ice, rain, snow, optionally graupel).

• The total mass fraction qn of each category is predicted. To accomplish this, the shapes and the size distributions of particles must be assumed and the microphysical processes must be parameterized in terms of qn and the other grid-scale variables

1 1 , , , , , ,n

n nqn

qnqP S F

qV q n i c v r s g

t z

KKKKKKKKKKKKKK

where Fqn are the turbulent fluxes (sub-grid scale), Sqn represent cloud microphysical sources and sinks, Pqn denotes the precipitation or sedimentation fluxes

Page 14: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

Microphysical Processes in COSMO model

Page 15: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

Cumulus Parameterization• A technique used in NWP to predict the collective effects of

convective clouds, that may exist within a single grid element, in terms of grid-scale properties

• Tiedtke scheme used in COSMO model can be grouped into the family of mass-flux schemes (use simple cloud model to simulate rearrangements of mass in a vertical column)

• In the Tiedke scheme a 1-dimensional cloud model is closed by making convection (triggering and intensity) dependent on the moisture supply by large-scale flow convergence and boundary layer turbulence (vertical distribution of heating and drying is estimated using the 1-D cloud model to satisfy the constraints on intensity)

• Column equilibrium is supposed for precipitation formed in convective clouds

Sqr includes the conversion of cloud water to form rain, the evaporation of rain in the downdraft and below the cloud base

10 r

rqqP

zS

Page 16: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

“Tiedke” scheme

Updraft

entrainment

and

detrainmentDowndraft

entrainment

and

detrainment

Cloud top detrainment

moisture convergence

Adapted from Baldwin (2001)

Page 17: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

Objective verification of COSMO-ME precipitation forecasts against SYNOP stations is routinely performed at CNMCA.6h, 12h and 24h accumulated precipitation scores are calculated for a three month period.

Objective Verification 

MAM (March, April,May) 2007

Page 18: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

Precipitation prediction is an example of a yes/no forecast. Some scores (FB, TS, ETS, FAR, etc.) are usually computed from the contingency table.

FB=(hits+false alarms)/(hits+misses)

The Frequency Bias (FB) measures the ratio of the frequency of forecast events to the frequency of observed events and indicates whether the forecast system has a tendency to underforecast (FB<1) or overforecast (FB>1) events (precipitation frequency).

TS=hits/(hits+false alarms+misses)

The Threat Score (TS) measures the fraction of observed and/or forecast events that were correctly predicted. The TS is somewhat sensitive to the climatology of the event, tending to give poorer scores for rare events. The Equitable Threat Score is designed to help offset this tendency.

ETS=(hits-hits expected by chance)/(hits+false alarms+misses–hits expected by chance)where hits expected by chance = (total forecasts of the event) * (total observations of the event) / (sample size)

Objective Verification 

Contingency Table

hits false

alarms

misses correct

negatives

forecast

observedyes no

yes

no

Page 19: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

Objective Verification24h Acc. Precipitation - FBI

Page 20: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

Objective Verification24h Acc. Precipitation - ETS

Page 21: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

Objective Verification12h Acc. Precipitation - FBI

Page 22: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

Objective Verification12h Acc. Precipitation - ETS

Page 23: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

Objective Verification06h Acc. Precipitation - FBI

Page 24: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

Objective Verification06h Acc. Precipitation - ETS

Page 25: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

COSMOME vs ECMWF MAM – FBI

Acc. Precipitation in 12h

Objective VerificationComparison with ECMWF

Page 26: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

COSMOME vs ECMWFMAM – ETS

Acc. Precipitation in 12h

Objective VerificationComparison with ECMWF

Page 27: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

QPF verification of the 4 model versions at 7 km res. (COSMO-I7, COSMO-7, COSMO-EU, COSMO-ME) with the 2 model versions at 2.8 km res. (COSMO-I2, COSMO-IT)

Specifications:

• Dataset: high resolution network of rain gauges coming from COSMO dataset and Civil Protection Department 1300 stations

• Method: 24h/6h averaged cumulated precipitation value over 90 meteo-hydrological basins

•Model selection: run 00UTC, D+1

Precipitation verification comparison in 2008/2009 among the several COSMO-Model versions (Elena Oberto, Massimo Milelli - ARPA Piemonte)

Presentation at COSMO general meeting 2009

Objective Verificationwith a high resolution raingauge network

Page 28: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

Seasonal trend (high thres)• Bias reduction trend, at least during last year

• Seasonal cycle: big peak during spring-summertime (convective period) seems to disappear during last summer (… why?)

• General good performance during last year

• Pronounced underestimation for Cosmo-7 during last seasons

From Oberto presentation at COSMO general meeting 2009

Objective Verification

Page 29: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

Seasonal trend (high thres)

• Slightly improvement trend

• Worse performance during summertime (except 2007)

From Oberto presentation at COSMO general meeting 2009

Objective Verification

Page 30: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

Future Developments

• In the CNMCA data assimilation system:– update error statistics in 3DVAR– assimilate new observations (NOAA-19 AMSUA

radiances, IASI and GRAS retrievals)– test LETKF (ensemble based) analysis algorithm– use high resolution SST and SWE analysis

• In COSMO-ME model:– test Runge-Kutta dynamical core– investigate changes in the cumulus parameterization

and microphysics scheme (to reduce the overestimation of small precipitation values during morning and noon and possibly to tune the onset of diurnal convection)

– enlarge integration domain and reduce grid spacing

Page 31: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

Future developments

During CDOP-1 the following improvements are foreseen: – extending the cover to the full H-SAF area. In order

not to affect the operational NWP activity at CNMCA, this will probably be implemented by decomposing the area in more frames;

– increase the number of runs/day. Currently, although the set of products (integrated over 3, 6, 12 and 24 h and precipitation rate) are disseminated every 3 hours, at synoptic times, they are generated by only two distinct runs/day. It is envisaged to move to 4 runs/day, in order to improve timeliness.

– improve the model resolution from the current 7 km to an extent to be assessed for cost/benefit

Page 32: HSAF Training on Precipitation Products, Rome, 14-15 December 2009 Precipitation Computed by COSMO-ME model (PR ASS1) Lucio TORRISI Italian Met. Service

HSAF Training on Precipitation Products, Rome, 14-15 December 2009

Thank you for your attention!