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Zentralanstalt für Meteorologie und Geodynamik Meteorologisch-Geophysikalisches Kolloquium: IMG-Wien 10.05.2011 Zentralanstalt für Meteorologie und Geodynamik Evaluation of the COSMO-CLM model simulations for the Alpine Region

Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

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Page 1: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011 Zentralanstalt für

Meteorologie

und Geodynamik

Evaluation of the COSMO-CLM

model simulations for the Alpine Region

Page 2: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 2 / 52

What you can expect from the next 45 minutes....

Climate models, climate modelling and our contribution at ZAMG(Ivonne Anders)

Model evaluation – quality and uncertainties of the model results(Klaus Haslinger)

Added value of increased spatial resolutions(Maja Zuvela Aloise)

Trends in observations and model data(Michael Hofstätter)

Summary and “message2go”(Michael Hofstätter)

Page 3: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 3 / 52

Climate models:

What is it? And how does it work?

FORCING CLIMATE MODEL OUTPUT

INP

UT

DA

TA

CLIM

AT

E

MO

DE

L

MO

DE

L O

UT

PU

T

Page 4: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 4 / 52

Climate models:

What is it? And how does it work?

NATURAL FORCING

• earth covered by plants reduce the green house gas – Concentration

• moving continents

• orbital forcings (Milanković cycles)

• sunspots

• vulcanic eruptions

• longlived greenhouse gases

• tropospheric sulphate

INPUT DATA

ANTHROPOGENIC FORCING

Page 5: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 5 / 52

Climate models:

What is it? And how does it work?

NATURAL FORCING

• earth covered by plants reduce the green house gas – Concentration

• moving continents

• orbital forcings (Milanković cycles)

• sunspots

• vulcanic eruptions

• longlived greenhouse gases

• tropospheric sulphate

INPUT DATA

ANTHROPOGENIC FORCING

Page 6: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 6 / 52

Climate models:

What is it? And how does it work?

FORCING CLIMATE MODEL OUTPUT

INP

UT

DA

TA

CLIM

AT

E

MO

DE

L

MO

DE

L O

UT

PU

T

Page 7: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 7 / 52

Climate models:

What is it? And how does it work?

Dynamical Models

Statistical ModelsGCM

RCM

AOGCM

ESM

LRMarkov Chain

weather generatorPCA

INPUT DATACLIMATE MODEL

numerical representations of various parts

of the Earth's climate system

statistical relationship between

large scale and local processes

… …

Page 8: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 8 / 52

Climate models:

What is it? And how does it work?

Global Climate Models (GCM)

limitations of the GCMs on representation of large scale

effects on the global climate due to changes in GHG-

concentration, volcanos etc.

strongly simplified, but containing the most important

processes

horizontal resolutions 3° - 1.5°

CLIMATE MODEL

Page 9: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 9 / 52

Climate models:

What is it? And how does it work?

Regional Climate Models (RCM)

containing complex model physics and due to higher spatial

resolution they are able to reproduce local effects due to

orography or land use

using Model output from GCMs as forcing

horizontal resolution 50 – 3km (0.5° - 0.025°)

CLIMATE MODEL

Page 10: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 10 / 52

Climate models:

What is it? And how does it work? CLIMATE MODEL

Horizontal Resolutions - Grids

Page 11: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 11 / 52

Climate models:

What is it? And how does it work? CLIMATE MODEL

Vertical Resolutions - Levels

Page 12: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 12 / 52

Climate models:

What is it? And how does it work? CLIMATE MODEL

Vertical Resolutions - Levels

hybrid levels

terrain following sigma-coordinates

Page 13: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 13 / 52

Climate models:

What is it? And how does it work? CLIMATE MODEL

Subscale Processes - Parameterizations

The problem with dividing the atmosphere into lots of little cubes is that there are

many processes that are smaller than the cubes!

Models include lots of parameterization s to

describe the processes

e.g. how much cloud is there..

Page 14: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 14 / 52

Climate models:

From large to small spatial scales and from long to short time scales ...

1s 1min 1hour 1year 1000years 1Mio years 100Mio years

1cm

1m

1km

1000 km

100000 km

1day

micro

turbulence

boundary

layer

turbulence

cumulus

convection

thunder

storms

cloud

clusters

cyclones

planetary

waves

inclination

solar variability

and

vulcanos

small ice age

orbital

forcings

{

CLIMATE MODEL

Page 15: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 15 / 52

Climate models:

From large to small spatial scales and from long to short time scales ...

1s 1min 1hour 1year 1000years 1Mio years 100Mio years

1cm

1m

1km

1000 km

100000 km

1day

micro

turbulence

boundary

layer

turbulence

cumulus

convection

thunder

storms

cloud

clusters

cyclones

planetary

waves

inclination

solar variability

and

vulcanos

small ice age

orbital

forcings

{Global Climate Models

CLIMATE MODEL

Page 16: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 16 / 52

Climate models:

From large to small spatial scales and from long to short time scales ...

1s 1min 1hour 1year 1000years 1Mio years 100Mio years

1cm

1m

1km

1000 km

100000 km

1day

micro

turbulence

boundary

layer

turbulence

cumulus

convection

thunder

storms

cloud

clusters

cyclones

planetary

waves

inclination

solar variability

and

vulcanos

small ice age

orbital

forcings

{Global Climate ModelsRegional Climate

Models

CLIMATE MODEL

Page 17: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 17 / 52

Climate models:

What is it? And how does it work?

FORCING CLIMATE MODEL OUTPUT

INP

UT

DA

TA

CLIM

AT

E

MO

DE

L

MO

DE

L O

UT

PU

T

Page 18: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 18 / 52

Climate models:

What is it? And how does it work?

FORCING CLIMATE MODEL OUTPUT

INP

UT

DA

TA

CLIM

AT

E

MO

DE

L

MODEL OUTPUT

Results for every grid box,

at different pressure levels or at surface

2D- und 3D- arrays, up to hourly

Page 19: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 19 / 52

Climate models:

The Regional Climate Model COSMO-CLM

• non-hydrostatic limited-area Modell

• based on the forecast model of DWD (German Weather Service)

• incl. soil model „Terra-ML“ and lake model „FLake“

• Community Model

COSMO- CLM Community

www.clm-community.euCOSMO – Dynamics and Physics

http://www.cosmo-model.org/content/model/

documentation/core/default.htmMeteorologische Zeitschrift

Special Issue, Vol. 17, 2008

Page 20: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 20 / 52

1st nesting step

Climate models:

The simulations we carried out at ZAMG and the validation is about ...

50km

ERA40

Reanalysis Data

1958-2002

150km

T,U,V,QV,..

Page 21: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 21 / 52

Climate models:

The simulations we carried out at ZAMG and the validation is about ...

50km

ERA40

Reanalysis Data

2002

150km

T,U,V,QV,..

1st nesting step

T,U,V,QV,..

2nd nesting step

10km

Page 22: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 22 / 52

Climate models:

The simulations we carried out at ZAMG and the validation is about ...

50km

T,U,V,QV,..

2nd nesting step

10km

T,U,V,QV,..

3rd nesting step

4km

Page 23: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 23 / 52

Climate models:

Can I use my home computer for carrying out simulations? (the technical side of the topic)

Page 24: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 24 / 52

Climate models:

Can I use my home computer for carrying out simulations? (the technical side of the topic)

Example of a high performance computer for climate

modelling at the DKRZ in Hamburg.

http://www.dkrz.de

tape robot system

Installing the IBM HPC system

Page 25: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 25 / 52

Climate models:

Can I use my home computer for carrying out simulations? (the technical side of the topic)

• Cluster of 2 vektor nodes

• 16 CPUs (8 CPU per node)

• 128 Gbyte RAM

• 2 x 310 GB/s Memory band width

• 512 Gigaflops

(cp. Earth Simulator: 80x)

NEC SX-8REurope in 50km x 50km

Alps in 10km x 10km

1 simulated month

runs 17 minutes at 8CPU

1 simulated month

runs 60 minutes minutes

at 8CPU

Page 26: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 26 / 52

What you can expect from the next 15 minutes....

Climate models, climate modelling and our contribution at ZAMG(Ivonne Anders)

Model evaluation – quality and uncertainties of the model results(Klaus Haslinger)

Added value of increased spatial resolutions(Maja Zuvela Aloise)

Trends in observations and model data(Michael Hofstätter)

Summary and “message2go”(Michael Hofstätter)

Page 27: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 27 / 52

Evaluation of the 10km CCLM hindcast

Evaluation – what does that mean?

Datenset Period Parameter Temporal Res. Spatial Res. Domain Reference

CRU TS 1.2 1901-2000 T, Tx, Tn, P Monthy 10' Europe Mitchell et al., 2003

E-OBS 1950-2006 T, Tx, Tn, P Daily 0.22° Europe Haylock et.al., 2008

GPCC4 1901-2007 P Daily 18km Europe Schneider et al., 2008

HISTALP 1780-2007 T Monthly 5' GAR Chimani et al., 2010 (subm.)

HISTALP 1800-2000 P Monthly 5' GAR Chimani et al., 2010 (subm.)

STARTCLIM 1950-2005 T, P, S Daily 1km Austria Schöner et.al., 2003

Evaluation is systematic determination of merit, worth, and significance of something (the

Regional Climate Model COSMO-CLM) or someone using criteria against a set of

standards (different observation datasets).

Observation data:

Page 28: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 28 / 52

Evaluation of the 10km CCLM hindcast

Mean Bias (50km European Domain)

-5 -4 -3 -2 -1 -0.5 0.5 1 2 3 4 5

Mean seasonal bias in 2m temperature [K], CCLM-CRU, 1961-2000

Page 29: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 29 / 52

Evaluation of the 10km CCLM hindcast

Mean Bias (50km European Domain)

-150 -60 -20 20 60 150

Mean seasonal bias in precipitation sum [%], CCLM-CRU, 1961-2000

Page 30: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 30 / 52

Evaluation of the 10km CCLM hindcast

Mean Bias (GAR)

Mean seasonal bias in precipitation sum [%], CCLM-HISTALP, 1961-2000

Mean seasonal bias in 2m temperature [K], CCLM-EOBS, 1961-2000

Page 31: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 31 / 52

Evaluation of the 10km CCLM hindcast

Correlation (GAR)

Correlation of seasonal 2m temperature mean, CCLM-HISTALP, 1961-2000

Co

rre

latio

n

Altitude [m]

Page 32: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 32 / 52

Evaluation of the 10km CCLM hindcast

Correlation (GAR)

Correlation of seasonal precipitation sum, CCLM-HISTALP, 1961-2000

Co

rre

latio

n

Altitude [m]

Page 33: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 33 / 52

Evaluation of the 10km CCLM hindcast

Annual Cycles (Austria)

Mean annual cycle of precipitation for five climatic regions in Austria, CCLM-STARTCLIM, 1961-2000

Page 34: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 34 / 52

Mean annual cycle of standard deviation of precipitation for five climatic regions in Austria,

CCLM-STARTCLIM, 1961-2000

Evaluation of the 10km CCLM hindcast

Annual Cycles (Austria)

Page 35: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 35 / 52

Evaluation of the 10km CCLM hindcast

Bias in Extremes and Derived Indices (Austria)

Mean seasonal bias of the precipitation sum above the 98th percentile [mm], CCLM-STARTCLIM, 1961-2000

Mean bias of the simple daily intensity index [mm/d],

CCLM-STARTCLIM, 1961-2000

Mean bias of number of days with RR > 1mm [d],

CCLM-STARTCLIM, 1961-2000

Page 36: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 36 / 52

What you can expect from the next 12 minutes....

Climate models, climate modelling and our contribution at ZAMG(Ivonne Anders)

Model evaluation – quality and uncertainties of the model results(Klaus Haslinger)

Added value of increased spatial resolutions(Maja Zuvela Aloise)

Trends in observations and model data(Michael Hofstätter)

Summary and “message2go”(Michael Hofstätter)

Page 37: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 37 / 52

CCLM Simulation for Austria: 4 km resolution

(1) Is there a value added by the dynamical downscaling to finer resolution?

(2) How good are the climate model simulations compared to the observational analysis model?

(3) Can we compare the climate model results directly with the observations at the stations?

10 km 4 km

Page 38: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 38 / 52

Comparison CCLM 10 km vs. 4 km: Temperature bias

Observational dataset: STARTCLIM 1 km gridded daily mean temperature

Period: 1961-2000

(1) similar spatial patterns: cold bias in the mountain region

(2) mean bias is not reduced

10 km 4 km

http://www.zamg.ac.at/forschung/klimatologie/klimawandel/StartClim2007.A/

Page 39: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 39 / 52

Comparison CCLM 10 km vs. 4 km: Temperature

(1) no significant differences in temperature distributions on seasonal basis

(2) small improvement in temperature correlation in winter period

4 km

10 km

Temperature frequency distribution

Page 40: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 40 / 52

10 km 4 km

Comparison CCLM 10 km vs. 4 km: Precipitation bias

Observational dataset: STARTCLIM 1 km gridded daily precipitation sum

Period: 1961-2000

(1) similar spatial patterns: overestimation of precipitation in the mountain region

(2) mean bias is not reduced

http://www.zamg.ac.at/forschung/klimatologie/klimawandel/StartClim2007.A/

Page 41: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 41 / 52

Comparison CCLM 10 km vs. 4 km: Precipitation

(1) small differences in precipitation distributions on seasonal basis

(2) no significant reduction of bias

4 km

10 km

Precipitation frequency distribution

Page 42: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 42 / 52

Comparison CCLM (4 km) vs. INCA (1 km): Wind speed maximum

Strong wind days: Number of days where daily maximum wind speed > 10.5 m/s

(1) similar horizontal patterns

(2) difference in resolution and time period

(Haiden et al., 2011)

http://www.zamg.ac.at/incaanalyse/

1980-2002 2003-2010

Page 43: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 43 / 52

Lowland Valley Mountain

m/s m/s m/s

Comparison CCLM (4 km), INCA (1 km), Observations: Wind speed

Wind speed distribution at the stations:

(1) Lowland: good agreement

(2) Valley: station dependant

(3) Mountain: underestimation of wind speeds

Page 44: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 44 / 52

Neighbouring points

Vertical levels

Comparison CCLM (4 km) vs. station data: Wind speed

Wind speed distribution at the stations compared to:

(1) Neighbouring points in the model: possible improvement

(2) Vertical levels: better agreement for the mountain stations

Page 45: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 45 / 52

Comparison CCLM (4 km) vs. stations: Wind speed

QQ-Plot: Percentiles of wind speed at the stations compared to the model

Good agreement

Overestimation

Non-linear bias

Underestimation

Page 46: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 46 / 52

What you can expect from the next 7 minutes....

Climate models, climate modelling and our contribution at ZAMG(Ivonne Anders)

Model evaluation – quality and uncertainties of the model results(Klaus Haslinger)

Added value of increased spatial resolutions(Maja Zuvela Aloise)

Trends in observations and model data (10km Hindcast GAR)(Michael Hofstätter)

Summary and “message2go”(Michael Hofstätter)

Page 47: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 47 / 52

Evaluation of the 10km CCLM hindcast GAR-Regions

Summer precipitation (JJA): Floating Trend Analysis (15y) 1961-2000

CL

MH

ista

lp

Decadal variability

CONCURRENT but OVERESTIMATED

in terms of magnitude!

Offset: +150mm

Page 48: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 48 / 52

Evaluation of the 10km CCLM hindcast GAR

Temperature 2m: Floating Trend Analysis (15y) 1961-2000

CL

MH

ista

lp

?

Page 49: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 49 / 52

Evaluation of the 10km CCLM hindcast

Trends (GAR)

CC

LM

HIS

TA

LP

Seasonal trends in 2m temperature [K], 1961-2000

+

+

+

Page 50: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 50 / 52

+0.2°

-0.7°

+1.2°

+1.8°

+1.5° +1.5°

+2.2°+2.2°

Trend dependency on height – T2m (AT 1961-2000)

Page 51: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 51 / 52

Uncertainty of observations GAR:

mean

pre

cip

itati

on

> 8

00m

(m

m/y

)

(a)

(b)

(a) mean precipitation > 800m (mm/year)

∆ = 0-100mm

(b) Range of mean monthly precipitation (1961-2000)

between OBS datasets⓿

Which OBS-dataset to choose?

Page 52: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011

Evaluation of the COSMO-CLM

model simulations for the Alpine regionFolie 52 / 52

CCLM Simulation for Austria: some CONCLUSIONS 2 go

(1) CCLM shows reasonable skill in certain processes in the Alpine Region

(2) Is there an added value downscaling from 10km to 4km ?

no significant bias reduction can be detected, similar bias with finer spatial structures

(3) We see RCM simulations are currently at their limits at 10km in the Alpine Region

furthermore gridded OBS with effective resolution .lt. 10km are missing.

(4) Future aspects: boundary layer processes, surface/soil parametrization, coupled Mediterranean Sea,..

(5) One model strategy: when focus is on specific processes (selective optimisations)

(6) Multi model strategy: for conventional climate change scenarios (uncertainty estimates!)

Page 53: Evaluation of the COSMO-CLM model simulations for … · micro turbulence boundary layer turbulence cumulus convection thunder storms cloud clusters cyclones planetary waves ... Evaluation

Zentralanstalt für Meteorologie und Geodynamik

Meteorologisch-Geophysikalisches

Kolloquium: IMG-Wien

10.05.2011 Zentralanstalt für

Meteorologie

und Geodynamik

Regional Climate

Change Scenarios

Urban Climate

Simulations

Variability, Extremes and

Uncertainty Analysis

Climate Simulations for

Impact Research