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Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss Priority project « Advanced interpretation and verification of very high resolution models »

Priority project « Advanced interpretation and verification of very high resolution models »

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Priority project « Advanced interpretation and verification of very high resolution models ». Topics. Advanced postprocessing of weather parameters Verification of very high resolution models, incl. fuzzy verification methods Hydrological applications. 3. Hydrological applications. - PowerPoint PPT Presentation

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Page 1: Priority project « Advanced interpretation and verification of very high resolution models »

Federal Department of Home Affairs FDHAFederal Office of Meteorology and Climatology MeteoSwiss

Priority project « Advanced interpretation and verification

of very high resolution models »

Page 2: Priority project « Advanced interpretation and verification of very high resolution models »

2 COSMO General meeting ¦ Cracow, September 2008Pierre.Eckert[at]meteoswiss.ch

Topics

1. Advanced postprocessing of weather parameters

2. Verification of very high resolution models, incl. fuzzy verification methods

3. Hydrological applications

Page 3: Priority project « Advanced interpretation and verification of very high resolution models »

3 COSMO General meeting ¦ Cracow, September 2008Pierre.Eckert[at]meteoswiss.ch

3. Hydrological applications

Hydrology (precipitation adaptation):

Presentation by A. Mazur

Snow parametrisation:

Presentation by E. Machulskaya

Page 4: Priority project « Advanced interpretation and verification of very high resolution models »

4 COSMO General meeting ¦ Cracow, September 2008Pierre.Eckert[at]meteoswiss.ch

1. Recognition of weather elements

• Done last year: recognition of thunderstorms with the boosting algorithm:

• Choice of predictors

Perler, Kohli, Walser

Page 5: Priority project « Advanced interpretation and verification of very high resolution models »

5 COSMO General meeting ¦ Cracow, September 2008Pierre.Eckert[at]meteoswiss.ch

1. Kalman filtering of COSMO LEPS

V. Stauch, poster outside

Page 6: Priority project « Advanced interpretation and verification of very high resolution models »

6 COSMO General meeting ¦ Cracow, September 2008Pierre.Eckert[at]meteoswiss.ch

2. Verification of very high resolution models

Goals

• 1-3 km scale (VHR)• Focus on precipitation• Is VHR (~2km) better than HR (~7km)?• Model intercomparison• Generate products related to the verification• Way to define the scores could depend on the

application (value)• Use synop, (high resolution rainguage network),

radar, evt. composition of all (gridded observations)

Page 7: Priority project « Advanced interpretation and verification of very high resolution models »

7 COSMO General meeting ¦ Cracow, September 2008Pierre.Eckert[at]meteoswiss.ch

Which rain forecast would you rather use?

Mesoscale model (5 km) 21 Mar 2004

Sydney

Global model (100 km) 21 Mar 2004

Sydney

Motivation

Observed 24h rain

RMS=13.0 RMS=4.6

B. Ebert

Page 8: Priority project « Advanced interpretation and verification of very high resolution models »

8 COSMO General meeting ¦ Cracow, September 2008Pierre.Eckert[at]meteoswiss.ch

Motivation: precipitation pattern

7km

2km

Page 9: Priority project « Advanced interpretation and verification of very high resolution models »

9 COSMO General meeting ¦ Cracow, September 2008Pierre.Eckert[at]meteoswiss.ch

Fuzzy Verification F. Ament

Verification on coarser scales than model scale: “Do not require a point wise match!“

X XX X

X Xx XXX

x

Method Raw Data Fuzzyfication Score Example result

Upscaling

Average

Equitable threat score

Fraction Skill

Score (Roberts and Lean, 2005)

Fractional coverage

Skill score with reference to

worst forecast

X XX X

X Xx XXX

x

Page 10: Priority project « Advanced interpretation and verification of very high resolution models »

10 COSMO General meeting ¦ Cracow, September 2008Pierre.Eckert[at]meteoswiss.ch

Expected behaviour of scores

From Nigel Roberts (2005)

Page 11: Priority project « Advanced interpretation and verification of very high resolution models »

11 COSMO General meeting ¦ Cracow, September 2008Pierre.Eckert[at]meteoswiss.ch

Application of scores to a perfect forecast

All scores should equal !

But, in fact, 5 out of 12 do not!

Page 12: Priority project « Advanced interpretation and verification of very high resolution models »

12 COSMO General meeting ¦ Cracow, September 2008Pierre.Eckert[at]meteoswiss.ch

Requested theoretical properties of scores

Avoid « leaking » scores Use illustrative and understandable scores Score should give a real information of the forecast

quality on the different scales Monotonic behavior concerning

• scale (best values for large scales)• frequency of occurrence (best values for high

frequencies of occurrence) Represent some significant characteristics of the PDF

(obs and forecast)

Page 13: Priority project « Advanced interpretation and verification of very high resolution models »

13 COSMO General meeting ¦ Cracow, September 2008Pierre.Eckert[at]meteoswiss.ch

Requested practical properties of scores

Agreement between subjective and objective judgment

Possible help in decision making Correspond to the needs of the users Should be able to provide a comparison between 2km

and 7 km models (also global models) Should not use a matching between prediction and

observation because it would not allow the generation of univocal products

Page 14: Priority project « Advanced interpretation and verification of very high resolution models »

14 COSMO General meeting ¦ Cracow, September 2008Pierre.Eckert[at]meteoswiss.ch

Chosen scores

Our best candidates:

Upscaling and Fraction skill score

Corresponding products

• Upscaling mean around a point / station• Fraction skill score probability to exceed some

threshold in a neighbourhood

Page 15: Priority project « Advanced interpretation and verification of very high resolution models »

15 COSMO General meeting ¦ Cracow, September 2008Pierre.Eckert[at]meteoswiss.ch

Sp

atia

l sca

le (

km)

Sp

atia

l sca

le (

km)

Fuzzy Verification: COSMO-DE – COSMO-EU

90

58

33

20

7

90

58

33

20

7

goodbad

Threshold (mm/3h) Threshold (mm/3h) Threshold (mm/3h)

- =

Fra

ctio

n sk

ill s

core

Ups

calin

g

=-COSMO-EU (7km)COSMO-DE (2.8km) Difference

COSMO-EU better COSMO-DE better

JJA 2007, Verification against Swiss Radar Composite, 3 hourly accumulations

Page 16: Priority project « Advanced interpretation and verification of very high resolution models »

16 COSMO General meeting ¦ Cracow, September 2008Pierre.Eckert[at]meteoswiss.ch

Sp

atia

l sca

le (

km)

Sp

atia

l sca

le (

km)

Fuzzy Verification COSMO-2 – COSMO-7

90

58

33

20

7

90

58

33

20

7

goodbad

Threshold (mm/3h) Threshold (mm/3h) Threshold (mm/3h)

- =

Fra

ctio

n sk

ill s

core

Ups

calin

g

=-COSMO-7 (7km)COSMO-2 (2.2km) Difference

COSMO-7 better COSMO-2 better

JJA 2007, Verification against Swiss Radar Composite, 3 hourly accumulations

Page 17: Priority project « Advanced interpretation and verification of very high resolution models »

17 COSMO General meeting ¦ Cracow, September 2008Pierre.Eckert[at]meteoswiss.ch

Monthly dependencycut-off 03h, accumulation 03h

COSMO-DE -

COSMO-EU

June

COSMO-2-

COSMO-7

July

August

Page 18: Priority project « Advanced interpretation and verification of very high resolution models »

18 COSMO General meeting ¦ Cracow, September 2008Pierre.Eckert[at]meteoswiss.ch

Quarterly summaries of „Fuzzy“-scores

FSS Autumn 2007

U. Damrath

Page 19: Priority project « Advanced interpretation and verification of very high resolution models »

19 COSMO General meeting ¦ Cracow, September 2008Pierre.Eckert[at]meteoswiss.ch

Monthly summaries of „Fuzzy“-scores

FSS July 2007

Page 20: Priority project « Advanced interpretation and verification of very high resolution models »

2020

Analysis of precipitation in boxesAnalysis of precipitation in boxes

Average number of stations in each area

( SON 2007)

X

We devised a verification methodology by aggregating observed and predicted precipitation in boxes of 1°x 1°(labelled boxes in the map)

The choice of the size and position of the areas has been performed according to different rules:

• boxes have to be enough large in order to contain a high number of observation points (ranging from 20 to over 100, depending on location and period of time considered)

• boxes have to be homogeneous as much as possible in terms of geographic-territorial characteristics

M.-S. TesiniM.-S. TesiniC. CacciamaniC. Cacciamani

Page 21: Priority project « Advanced interpretation and verification of very high resolution models »

2121

Box 2 aut2007Box 2 aut2007

25 mm/24

23 mm/24

19 mm/24

90th percentile of “climatological” pdf

Page 22: Priority project « Advanced interpretation and verification of very high resolution models »

2222

Consideration on “day-by-day” Consideration on “day-by-day” behaviour behaviour

• COSMO-I7 seems to be more realistic than ECMWF in reproducing the intra-box variability.

• However, COSMO-I7 presents both a large number of false alarms and high “spikes”. On the other hand, ECMWF presents a greater number of missed alarms, especially for high thresholds.

• According to most standard verification measures, COSMO-I7 forecast would have poor quality, but it might be very valuable to the forecaster since it provides information on the distribution and variability of the rain field over the considered region.

Page 23: Priority project « Advanced interpretation and verification of very high resolution models »

23 COSMO General meeting ¦ Cracow, September 2008Pierre.Eckert[at]meteoswiss.ch

Neighbourhood method P. Kaufmann

• Cylindrical neighbourhood with fading zone

• Settings at MeteoSwiss: • COSMO-7 (6.6 km):

rxy= 5, rf= 5, rt=3

• COSMO-2 (2.2 km): rxy=10, rf=10, rt=1

• Effective radius:• COSMO-7: ~50 km• COSMO-2: ~35 km

x

y

t

Page 24: Priority project « Advanced interpretation and verification of very high resolution models »

24 COSMO General meeting ¦ Cracow, September 2008Pierre.Eckert[at]meteoswiss.ch

12 July: high probabilities match well with precipitation pattern

24 h sum 06 – 06 UTC next day

Probability of 12 h sum above 35 mm

06 – 18 UTC

18 – 06 UTC

Page 25: Priority project « Advanced interpretation and verification of very high resolution models »

25 COSMO General meeting ¦ Cracow, September 2008Pierre.Eckert[at]meteoswiss.ch

15 August: high probabilities match well precipitation pattern

24 h sum 06 – 06 UTC next day

Probability of 12 h sum above 35 mm

06 – 18 UTC

18 – 06 UTC

Page 26: Priority project « Advanced interpretation and verification of very high resolution models »

26 COSMO General meeting ¦ Cracow, September 2008Pierre.Eckert[at]meteoswiss.ch

17 July: completely missed event

24 h sum 06 – 06 UTC next day

Probability of 12 h sum above 35 mm

06 – 18 UTC

18 – 06 UTC

Page 27: Priority project « Advanced interpretation and verification of very high resolution models »

27 COSMO General meeting ¦ Cracow, September 2008Pierre.Eckert[at]meteoswiss.ch

Conclusionson verification of very high resoution models

• Results of Upscaling and Fraction skill score are reasonable.• Scores increase with box size, but it is difficult to extract

optimal size by looking at one single model.• Overall better results for very high-res models• This benefits of very high-res models is rather to see in

situations where precipitation variability is large: convection , orography, summer…

• …and at scales of 30 to 50 km• Products can be generated

• Regional means (not new)• Probability to exceed threshold in neighborhood• Or possibly the whole pdf?