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Eidgenössisches Departement des Innern EDI Bundesamt für Meteorologie und Klimatologie MeteoSchweiz On the 2m temperature and dew point diagnostics in the COSMO model Matteo Buzzi and M.W. Rotach MeteoSwiss

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Page 1: On the 2m temperature and dew point diagnostics in the COSMO … · 2016. 12. 20. · On the 2m temperature diagnostics in the COSMO model | matteo.buzzi@meteoswiss.ch 8 Unrealistic

Eidgenössisches Departement des Innern EDIBundesamt für Meteorologie und Klimatologie MeteoSchweiz

On the 2m temperature and dew point diagnostics in the

COSMO model

Matteo Buzzi and M.W. Rotach MeteoSwiss

Page 2: On the 2m temperature and dew point diagnostics in the COSMO … · 2016. 12. 20. · On the 2m temperature diagnostics in the COSMO model | matteo.buzzi@meteoswiss.ch 8 Unrealistic

2On the 2m temperature diagnostics in the COSMO model | [email protected]

Overview

• Introduction• Surface layer• Operational 2m temperature and dew point diagnostics

• Possible sources of error• The role of subgrid scale orography

• Alternatives: new interpolation formulas or profiles• Case studies

• Intercomparison: verification results• Conclusions

Page 3: On the 2m temperature and dew point diagnostics in the COSMO … · 2016. 12. 20. · On the 2m temperature diagnostics in the COSMO model | matteo.buzzi@meteoswiss.ch 8 Unrealistic

3On the 2m temperature diagnostics in the COSMO model | [email protected]

Surface layer

0

Inertial sublayer (ISL)

Roughness sublayer (RSL)

hcan

z*

0.1zi

Θ'w' sensible heat fluxQv'w' latent heat flux

Θ'w'surf or Qv'w'surf

constant turbulent fluxes

inconstant fluxes

NWP modelsfirst model layer

2m

z*= 2hcan

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4On the 2m temperature diagnostics in the COSMO model | [email protected]

COSMO 2m temperature and dew point diagnostics: 3 cases

T(ke), Q(ke)

H1=z0

0Ts,Qs

H2=z0+h(ke)

z0+h(ke-1) T(ke-1), Q(ke-1)

hcan

skin

laye

r!

EXP LOG LOG INTERP

( ) ⎟⎟⎠

⎞⎜⎜⎝

⎛ ++= H

lam

Htur

HlamH

turH

lamcan rrrrrRCh log

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5On the 2m temperature diagnostics in the COSMO model | [email protected]

2m temperature: possible sources of error

• Surface temperature:• soil model (surface energy balance, LH, SH, GF, SWbal, LWbal)

• Atmosphere temperature:• dynamics (e.g. advection), convection, turbulence scheme

• Interpolation profile in the diagnostics:• choice of “wrong” profile function

• Surface description:• Roughness length:

• canopy height

Page 6: On the 2m temperature and dew point diagnostics in the COSMO … · 2016. 12. 20. · On the 2m temperature diagnostics in the COSMO model | matteo.buzzi@meteoswiss.ch 8 Unrealistic

6On the 2m temperature diagnostics in the COSMO model | [email protected]

COSMO-7 roughness length (7 km)[m]

Page 7: On the 2m temperature and dew point diagnostics in the COSMO … · 2016. 12. 20. · On the 2m temperature diagnostics in the COSMO model | matteo.buzzi@meteoswiss.ch 8 Unrealistic

7On the 2m temperature diagnostics in the COSMO model | [email protected]

COSMO-7 roughness length: local and orographic component (7 km)

z0 = z0, loc + z0,oro

z0, loc z0,oro[m] [m]

hcan

Page 8: On the 2m temperature and dew point diagnostics in the COSMO … · 2016. 12. 20. · On the 2m temperature diagnostics in the COSMO model | matteo.buzzi@meteoswiss.ch 8 Unrealistic

8On the 2m temperature diagnostics in the COSMO model | [email protected]

Unrealistic canopy height (7km)20.12.2006 6 UTC 20.12.2006 12 UTC [m]

exp profile is too often used!

hcan =z0, loc

0.1

( ) ⎟⎟⎠

⎞⎜⎜⎝

⎛ ++= H

lam

Htur

HlamH

turH

lamcan rrrrrRCh log

Page 9: On the 2m temperature and dew point diagnostics in the COSMO … · 2016. 12. 20. · On the 2m temperature diagnostics in the COSMO model | matteo.buzzi@meteoswiss.ch 8 Unrealistic

9On the 2m temperature diagnostics in the COSMO model | [email protected]

Averaged diurnal cycle: 15.04.2007

z0,oro< 0.2 m 0.2 m < z0,oro< 0.5 m

COSMO-7 over the alpine region

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10On the 2m temperature diagnostics in the COSMO model | [email protected]

Phase error

26.07.2007 COSMO-7- Swiss SYNOP stations

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11On the 2m temperature diagnostics in the COSMO model | [email protected]

Comparison of different diagnosticsProblem:

2 m temperature is too close to the surface temperatureSolution:

introduction of a local roughness length and try others diagnostics0. Introduce a realistic hcan in operational diagnostics

• But inconsistent with resistances (option only possible if surface transfer scheme and turbulence scheme are called twice)

1. Use a simple logarithmic interpolation as used for wind (newlog)• But not consistent with RSL (z0,loc >0.2m)!

2. ECMWF IFS diagnostics (logarithmic interpolation based on Monin-Obuchov similarity) (ecmwf)• But not consistent with RSL (z0,loc >0.2m)!

3. New approach (new):• New logarithmic profile (as 1.) only for gridcells with z0,loc < 0.2m• z0,loc > 0.2m new RSL profiles independent from surface

temperature4. Diagnostics for a SYNOP garden (by Matthias R.) (dwdnew)

• But not consistent with RSL (z0,loc >0.2m)!5. As 4. but with z0,loc instead of typical SYNOP z0 (dwdnew z0loc)

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12On the 2m temperature diagnostics in the COSMO model | [email protected]

H2 = H(ke) + z0, loc + d

New profiles: general aspects

0

Inertial sublayer ISL

Roughness sublayer RSL

hcan

z*

0.1zi

Temperature

T*, ISL fluxes

hcan =z0, loc

0.1z* = 2hcan

d =23

hcan

Approach for large z0,loc: derive temperature and specific humidity profile from turbulent flux profiles and atmospheric values

First model atmospheric levelH2

d

T,QV,H0,LH0, Mo0

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13On the 2m temperature diagnostics in the COSMO model | [email protected]

New profiles: 3 cases

newlog

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14On the 2m temperature diagnostics in the COSMO model | [email protected]

New profiles: formulationdθdz

=θ*(z)

α ⋅ (z − z0, loc )

θ*(z) =w'θ '(z)u*(z)

=w'θ '(z)

u'w'(z)2 + v'w'(z)2( )1 / 4

θ(z) = θ(z*) −θ*(z)

α ⋅ (z − z0, loc )dz

z0

z

θ*(z*)α ⋅ (z* − z0, loc )

= φhθ*

k(z* − d)⇒ α =

k(z* − z0, loc )φh (z* − d)

φh ( zL

)

Profile matching at z*

RSL: local scaling

Integration

ISLRSL

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15On the 2m temperature diagnostics in the COSMO model | [email protected]

Sensible heat flux and vertical temperature derivative

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16On the 2m temperature diagnostics in the COSMO model | [email protected]

Temperature and specific humidity

Page 17: On the 2m temperature and dew point diagnostics in the COSMO … · 2016. 12. 20. · On the 2m temperature diagnostics in the COSMO model | matteo.buzzi@meteoswiss.ch 8 Unrealistic

17On the 2m temperature diagnostics in the COSMO model | [email protected]

Case studies and model settings

• 5 cases 24h forecast COSMO 7km (fairly good weather)• 20.12.2006, 15.04.2007, 18.06.2006, 26.07.2007,

15.10.2007• COMSO 3.20, Runge-Kutta, IFS Analysis as BC, COSMO

analysis as IC• Verification with SYNOP stations for the domain covering

the alpine region (COSMO-2) (for all 6 variants)

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18On the 2m temperature diagnostics in the COSMO model | [email protected]

Variants compared with operational diagnostics

1. Simple logarithmic interpolation as used for wind (newlog)

2. ECMWF IFS diagnostics (ecmwf)

3. New approach (new): RSL profiles z0,loc > 0.2m

4. Diagnostics for a SYNOP garden (dwdnew)

5. As 4. but with z0,loc instead of typical SYNOP z0 (dwdnew z0loc)

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19On the 2m temperature diagnostics in the COSMO model | [email protected]

Results: diurnal cycle 15.04.2007

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20On the 2m temperature diagnostics in the COSMO model | [email protected]

Averaged diurnal cycle: 15.04.2007

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21On the 2m temperature diagnostics in the COSMO model | [email protected]

Comparison of the vertical profiles

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22On the 2m temperature diagnostics in the COSMO model | [email protected]

Comparison of the vertical profiles

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23On the 2m temperature diagnostics in the COSMO model | [email protected]

Verification: SYNOP alpine region 2m temperature 20.12.2006

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24On the 2m temperature diagnostics in the COSMO model | [email protected]

Verification: SYNOP alpine region2m dew point (RMSE)

Page 25: On the 2m temperature and dew point diagnostics in the COSMO … · 2016. 12. 20. · On the 2m temperature diagnostics in the COSMO model | matteo.buzzi@meteoswiss.ch 8 Unrealistic

25On the 2m temperature diagnostics in the COSMO model | [email protected]

2m temperature: results summary

RMSE[°C]

ME[°C]

STDEV ME[°C]

Operational 3.15 -0.86 3.03

new RSL 2.86 -0.62 2.79

newlog 2.74 -0.52 2.69

dwdnew 2.73 -0.44 2.70

dwdnew z0,loc 2.75 -0.56 2.69

ecmwf 2.74 -0.56 2.68

COSMO-7 verified on COMSO-2 domain (only 5 days)!

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26On the 2m temperature diagnostics in the COSMO model | [email protected]

Conclusions

• 2 m temperature and 2m dew point: multiple sources of error (soil, atmosphere, choice of the interpolation profile)

• Unrealistic canopy height (from subgridscale orography) is a significant source of error (choice between EXP and LOG profile)

• Operational diagnostics compared to 5 options based on local roughness length or on SYNOP garden

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27On the 2m temperature diagnostics in the COSMO model | [email protected]

Conclusions• Better verification results for all the 5 options:

• Phase shift improved• Cold bias in winter significantly reduced

but still important!• Logarithmic interpolation: the best results, BUT inconsistent

with the RSL (for z0,loc>0.2)!• The new RSL profiles perform comparably well and are

consistent with the RSL• Local roughness length necessary for diagnostics: should be

introduced in COSMO• Downscaling on a SYNOP garden:

• inconsistent with the mean gridbox conditions in the model• but gives better verification results (better SMA @ DWD)

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Eidgenössisches Departement des Innern EDIBundesamt für Meteorologie und Klimatologie MeteoSchweiz

Thank you for your attention!

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29On the 2m temperature diagnostics in the COSMO model | [email protected]

Verification: SYNOP Switzerland 2m temperature 20.12.2006

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30On the 2m temperature diagnostics in the COSMO model | [email protected]

New profiles: turbulent fluxes

u'w' = c ⋅ u'w'ISLz − z0zs − z0

⎛ ⎝ ⎜

⎞ ⎠ ⎟

2

exp a(1−z − z0zs − z0

⎛ ⎝ ⎜

⎞ ⎠ ⎟

⎝ ⎜

⎠ ⎟

v'w' = c ⋅ v'w'ISLz − z0zs − z0

⎛ ⎝ ⎜

⎞ ⎠ ⎟

2

exp a(1−z − z0zs − z0

⎛ ⎝ ⎜

⎞ ⎠ ⎟

⎝ ⎜

⎠ ⎟

u'w'(z*) = u'w'ISL v'w'(z*) = v 'w'ISL ⇒ c =z * −z0zs − z0

⎛ ⎝ ⎜

⎞ ⎠ ⎟

−2

exp a(1−z * −z0zs − z0

⎛ ⎝ ⎜

⎞ ⎠ ⎟

⎝ ⎜

⎠ ⎟

Momentum fluxes

Kaster-Klein and Rotach (2004)

Sensible heat flux

w'θ ' = w'θ 'ISLz − z0zs − z0

⎝ ⎜

⎠ ⎟

2

exp −ch zs − zzs

⎝ ⎜

⎠ ⎟

⎝ ⎜

⎠ ⎟ z < zs

w'θ ' = w'θ 'ISL z ≥ zs Modified from Christen (2005)

ch=1.2

a=2