atmosphere at rest experiments with the latest cosmo version and comparison with eulag

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Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss Atmosphere at rest experiments with the latest COSMO version and comparison with EULAG Oliver Fuhrer, MeteoSwiss

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Atmosphere at rest experiments with the latest COSMO version and comparison with EULAG. Oliver Fuhrer, MeteoSwiss. Introduction. Why again? experiments performed with EULAG, but different setup latest COSMO model version (4.14) more sensitivity studies What is tested? - PowerPoint PPT Presentation

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Page 1: Atmosphere at rest experiments with the latest COSMO version and comparison with EULAG

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

Atmosphere at rest experiments with the latest COSMO version and

comparison with EULAG

Oliver Fuhrer, MeteoSwiss

Page 2: Atmosphere at rest experiments with the latest COSMO version and comparison with EULAG

Introduction

• Why again?

- experiments performed with EULAG, but different setup

- latest COSMO model version (4.14)

- more sensitivity studies

• What is tested?

- terrain following coordinate transformation introduces additional truncation error term for flows which are nearly hydrostatic

- how large is this error?

• Basic setup

- topography

- u = v = w = 0

- hydrostatic equilibrium

Page 3: Atmosphere at rest experiments with the latest COSMO version and comparison with EULAG

Why does not everything cancel?

1

1 and BC determine p’ completely.

3

2

2 and 3 only cancel out to precision of discretization.

Page 4: Atmosphere at rest experiments with the latest COSMO version and comparison with EULAG

Ideal test case I

• 2-dimensional

• Schaer et al. MWR 2002 topography

• Gal-Chen coordinates

• ∆x = 1 km, Lx = 320 km

• ∆z = 400 m, Lz = 20 km

• ∆t = 10 s

• Reference atmosphereN = 0.01 s-1

• Initial stateT0 = 288.15 K, p0 = 105 Pa, dT/dlogp = 42

Page 5: Atmosphere at rest experiments with the latest COSMO version and comparison with EULAG

Sensitivity: Topography height

h = 0 m

h = 300 m

h = 1 m

h = 500 m

h = 10 m

h = 1000 m

h = 100 m

h = 2000 mh = 4000 m

Crash!!!

Page 6: Atmosphere at rest experiments with the latest COSMO version and comparison with EULAG

Sensitivity: Mountain Height

Page 7: Atmosphere at rest experiments with the latest COSMO version and comparison with EULAG

Sensitivity: Mountain Width

Page 8: Atmosphere at rest experiments with the latest COSMO version and comparison with EULAG

Sensitivity: Timestep

Page 9: Atmosphere at rest experiments with the latest COSMO version and comparison with EULAG

Sensitivity: Summary

• Mountain height / steepness play key role• Explicit vertical advection (EVA) helps• Timestep has small influence• θ or θ’ dynamics worsens situation• Independent of lower BC• Explicit hyper-diffusion on model levels helps• Time weighting (β) in fast-modes has no influence• Order of horizontal advection has negligible influence

Page 10: Atmosphere at rest experiments with the latest COSMO version and comparison with EULAG

Ideal test case II

• 2-dimensional

• Schaer et al. MWR 2002 topography

• Gal-Chen coordinates

• ∆x = 1 km, Lx = 320 km

• ∆z = 400 m, Lz = 20 km

• ∆t = 10 s

• Reference atmosphereN = 0.01 s-1

• Initial stateT0 = 288.15 K, p0 = 105 Pa, dT/dlogp = 42

• Rayleight sponge (> 13 km)

Page 11: Atmosphere at rest experiments with the latest COSMO version and comparison with EULAG

Sensitivity: Topography height

h = 0 m

h = 300 m

h = 1 m

h = 500 m

h = 10 m

h = 1000 m

h = 100 m

h = 2000 mh = 4000 m

Crash!!!

Crash!!!

Page 12: Atmosphere at rest experiments with the latest COSMO version and comparison with EULAG

Comparison COSMO vs. EULAG

2.0 10-12

1.8 10-5

1.0 10-4

2.2 10-4

4.5 10-4

6.0 10-3

(crash)

2.0 10-12

6.4 10-5

2.5 10-4

6.4 10-4

9.3 10-3

(crash)

(crash)

7.1 10-13

2.3 10-2

8.5 10-2

1.4 10-1

(crash)

(crash)

7.1 10-13

4.9 10-2

9.1 10-2

1.6 10-1

(crash)

(crash)

Page 13: Atmosphere at rest experiments with the latest COSMO version and comparison with EULAG

2.0 10-12

1.8 10-5

1.0 10-4

2.2 10-4

4.5 10-4

6.0 10-3

(crash)

2.0 10-12

6.4 10-5

2.5 10-4

6.4 10-4

9.3 10-3

(crash)

(crash)

7.1 10-13

2.3 10-2

8.5 10-2

1.4 10-1

(crash)

(crash)

7.1 10-13

4.9 10-2

9.1 10-2

1.6 10-1

(crash)

(crash)

Comparison EVA vs. IVA

1.8 10-12

2.0 10-5

1.1 10-4

2.4 10-4

4.7 10-4

6.3 10-3

2.9 10-1

1.8 10-12

7.1 10-5

2.7 10-4

6.6 10-4

1.1 10-2

3.1 10+1

(crash)

6.8 10-13

8.3 10-3

1.4 10-2

1.7 10-1

4.9 10-2

6.4 10-2

5.8 10-1

6.8 10-13

1.3 10-2

2.4 10-2

3.6 10-2

1.6 10-1

2.3 10+1

Page 14: Atmosphere at rest experiments with the latest COSMO version and comparison with EULAG

Conclusion

• Results with model version 4.14 are better than with model version 4.7

• Results for stable experiments compare well to EULAG and are always within one order of magnitude

• Model still crashes for too steep and high topography

• Explicit vertical advection (EVA) and some explicit hyper-diffusion go some way in stabilizing model, but do not solve problem

• Other factors have little or not influence