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Non-hydrostatic IFS at ECMWF

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Presentation on theme: "Non-hydrostatic IFS at ECMWF"— Presentation transcript:

1 Non-hydrostatic IFS at ECMWF
Mariano Hortal, Deborah Salmond, Agathe Untch, and Nils Wedi

2 Topics NH-IFS stability physics-dynamics coupling
NH-IFS climate and forecast performance Tracer transport: physics-dynamics coupling idealized flow experiments

3 NH-IFS Problem with horizontal diffusion, which lead to noise and model failure in the stratosphere.

4 Problem with horizontal diffusion
Inconsistency in setup of horizontal diffusion in NH at ECMWF: diffusion applied on horizontal divergence and the two new non-hydrostatic variables was different. This did not show up as a problem in CY30R1, however in CY31R1 it results in noise in the horizontal divergence: When the same diffusion is applied on the NH variables as on horizontal divergence this noise does not develop.

5 Model failure when coupled to the physics
Using large time-steps we encountered problems with “bull’s eyes” in the temperature field near the surface in areas with steep orographic gradients which lead to model failure.

6 2. Problem with temperature over steep orography
NH run at T159L60, ∆t=1h, NSITER=1 Temperature at level 59 after 27h

7 NH with NSITER=2, ∆t=1h Hydrostatic run, ∆t=1h (with physics)

8 NH with NSITER=1, ∆t=1h Hydrostat. with no phys, ∆t=1h (no physics)

9 Hydrostat. with no phys, ∆t=1h
NH with NSITER=1, ∆t=1h Hydrostat. with no phys, ∆t=1h LVERAVE_HLUV=FALSE (no physics)

10 2. Problem with temperature over steep orography
NH run at T159L91, NSITER=1, NEPHYS=3, Temperature at level 90 after 168h ∆t=0.5h ∆t=1h

11 Summary: near surface sensitivities in the vicinity of steep orography
Decrease the time-step Switching off the averaging of surface winds Change the number of iterations Sensitivity to pointwise large surface wind accelerations (implicit convection scheme formulation) LVERAVE_HLUV=F NSITER=2 works best!

12 Physics – Dynamics coupling
Development of 2 options to call physics: Call physics only in the last corrector step of the ICI scheme (adiabatic predictor steps) (NEPHYS=3), NH(3) Call physics in the predictor step and use these physical tendencies in each subsequent corrector step (NEPHYS=2), NH(2)

13 NH-IFS with physics Does the model climate of the NH version of IFS differ from the climate of the hydrostatic version for a Tl159L91 resolution ? 3 member ensemble 1 year daily SST forcing

14 zonal-mean zonal wind NH(3) – H(NH) H(NH) – H(IFS) NH(2)-H(NH) H(IFS)-ERA40

15 zonal-mean zonal temperature
NH(3) – H(NH) H(NH) – H(IFS) NH(2)-H(NH) H(IFS)-ERA40

16 NH H(NH) diff

17 Anomaly correlation and rms error: 12 cases, Tl159L91
NH H(NH) H 500hPa Z, Northern Hemisphere 500hPa Z, Southern Hemisphere 500hPa T, Tropics Anomaly correlation and rms error: 12 cases, Tl159L91 CPU time factor: H=1; H(NH)=1.5; NH=2; H(NH) and NH used NSITER=2

18 Physics – Dynamics coupling
2 separate calls to vertical diffusion scheme, before and after calls to cloud and convection to test possibility for a better near surface balance in the last corrector step of nonhydrostatic model hydrostatic test

19 Physics – Dynamics coupling
1 call to vdfmain 2 calls to vdfmain

20 Physics-Dynamics coupling Vertical diffusion
Anton Beljaars Physics-Dynamics coupling Vertical diffusion Negative tracer concentrations noticed despite a quasi-monotone advection scheme

21 Physics-Dynamics coupling Vertical diffusion
(Kalnay and Kanamitsu, 1988) Single-layer problem

22 Physics-Dynamics coupling Vertical diffusion
Two-layer problem depends on  !!!

23 (D+P)t (D+P)t+t  = 1.5 Dt+t  = 1 Anton Beljaars

24 Idealized flow past a mountain on the sphere
Initial zonal flow, isothermal atmosphere, no physics Hydrostatic mountain NL/U >>1 Non-hydrostatic mountain NL/U ~ 1 Froude number Nh/U ~1

25 Hydrostatic model Tl799L91, NL/U ~ 900 Hydrostatic regime Non-hydrostatic model Horizontal divergence D

26 Tl159L91, NL/U ~ 2.5 Near non-hydrostatic regime Horizontal divergence D hydrostatic model non-hydrostatic model

27 dt=3600s, sitra=100K dt=1800s, sitra=50K p-p_hyd noise dt=1800s, sitra=10K Blows up! dt=1800s, sitra=100K

28 dt=1800s, sitra=100K dt=1800s, sitra=150K dt=1800s, sitra=200K dt=1800s, sitra=350K Blows up!

29 Next steps Further investigate the physics-dynamics interaction with NH-IFS Test NH-IFS in higher resolution Idealized tests in the NH regime on the sphere Improve the scores …

30 dt=3600s, p-p_hyd dt=3600s, horiz. divergence dt=1800s, p-p_hyd dt=1800s, horiz. divergence


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