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ECMWF Governing Equations 1 Slide 1 Governing Equations I: reference equations at the scale of the continuum by Sylvie Malardel (room 10a; ext. 2414) after.

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Presentation on theme: "ECMWF Governing Equations 1 Slide 1 Governing Equations I: reference equations at the scale of the continuum by Sylvie Malardel (room 10a; ext. 2414) after."— Presentation transcript:

1 ECMWF Governing Equations 1 Slide 1 Governing Equations I: reference equations at the scale of the continuum by Sylvie Malardel (room 10a; ext. 2414) after Nils Wedi (room 007; ext. 2657) Thanks to Clive Temperton, Mike Cullen and Piotr Smolarkiewicz Recommended reading: An Introduction to Dynamic Meteorology, Holton (1992) An Introduction to Fluid Dynamics, Batchelor (1967) Atmosphere-Ocean Dynamics, Gill (1982) Numerical Methods for Wave Equations in Geophysical Fluid Dynamics, Durran (1999) Illustrations from Fondamentaux de Meteorologie, Malardel (Cepadues Ed., 2005)

2 ECMWF Governing Equations 1 Slide 2 Overview Introduction : from molecules to continuum Eulerian vs. Lagrangian derivatives Perfect gas law Continuity equation Momentum equation (in a rotating reference frame) Thermodynamic equation Spherical coordinates Averaged equations in numerical weather prediction models (Note : focus on dry (no water phase change) equations)

3 ECMWF Governing Equations 1 Slide 3 Note: Simplified view ! From molecules to continuum Newtons second law Boltzmann equations Navier-Stokes equations Euler equations individual particles statistical distribution continuum Mean free path number of particles kinematic viscosity ~1.x10 -6 m 2 s -1, water ~1.5x10 -5 m 2 s -1, air Mean value of the parameter Molecular fluctuations Mean value at the scale of the continuum Continuous variations

4 ECMWF Governing Equations 1 Slide 4 Perfect gas law The pressure force on any surface element containing M The temperature is defined as The link between the pressure, the temperature and the density of molecules in a perfect gas :

5 ECMWF Governing Equations 1 Slide 5 Perfect gas law : other forms or

6 ECMWF Governing Equations 1 Slide 6 Fundamental physical principles Conservation of mass Conservation of momentum Conservation of energy Consider budgets of these quantities for a control volume (a) Control volume fixed relative to coordinate axes => Eulerian viewpoint (b) Control volume moves with the fluid and always contains the same particles => Lagrangian viewpoint

7 ECMWF Governing Equations 1 Slide 7 Eulerian versus Lagrangian Eulerian : Evolution of a quantity inside a fixed box Lagrangian : evolution of a quantity following the particules in their motion

8 ECMWF Governing Equations 1 Slide 8 Eulerian vs. Lagrangian derivatives Particle at temperature T at position at time moves to in time. Temperature change given by Taylor series: i.e., then Let is the rate of change following the motion. total derivative local rate of change advection is the rate of change at a fixed point.

9 ECMWF Governing Equations 1 Slide 9 Sources vs. advection

10 ECMWF Governing Equations 1 Slide 10 Mass conservation Inflow at left face is. Outflow at right face is Difference between inflow and outflow is per unit volume. Similarly for y- and z-directions. Thus net rate of inflow/outflow per unit volume is = rate of increase in mass per unit volume = rate of change of density => Continuity equation (Eulerian point of view) Eulerian budget : Mass flux on left face Mass flux on right face

11 ECMWF Governing Equations 1 Slide 11 Mass conservation (continued) Continuity equation, mathematical transformation Continuity equation : Lagrangian point of view By definition, mass is conserved in a Lagrangian volume:

12 ECMWF Governing Equations 1 Slide 12 Momentum equation : frames Newtons Second Law in absolute frame of reference: N.B. use D/Dt to distinguish the total derivative in the absolute frame of reference. (1) We want to express this in a reference frame which rotates with the earth fixed star Rotating frame

13 ECMWF Governing Equations 1 Slide 13 Momentum equation : velocities = angular velocity of earth. For any vector = position vector relative to earths centre or Evolution in absolute frame Evolution in rotating frame

14 ECMWF Governing Equations 1 Slide 14 Momentum equation : accelerations Then from (1): In practice:

15 ECMWF Governing Equations 1 Slide 15 Momentum equation : Forces Forces - pressure gradient, gravitation, and friction Where = specific volume (= ), = pressure, = sum of gravitational and centrifugal force, = molecular friction, = vertical unit vector Magnitude of varies by ~0.5% from pole to equator and by ~3% with altitude (up to 100km).

16 ECMWF Governing Equations 1 Slide 16 Spherical polar coordinates (in the same rotating frame) : = longitude, = latitude, = radial distance Orthogonal unit vectors: eastwards, northwards, upwards. As we move around on the earth, the orientation of the coordinate system changes: Extra terms due to the spherical curvature

17 ECMWF Governing Equations 1 Slide 17 Components of momentum equation with

18 ECMWF Governing Equations 1 Slide 18 The shallow atmosphere approximation Shallowness approximation – For consistency with the energy conservation and angular momentum conservation, some terms have to be neglected in the full momentum equation. This approximation is then valid only if these terms are negligible. with

19 ECMWF Governing Equations 1 Slide 19 Energy conservation : Thermodynamic equation ( total energy conservation – macroscopic kinetic energy equation ) First Law of Thermodynamics: where I = internal energy, Q = rate of heat exchange with the surroundings W = work done by gas on its surroundings by compression/expansion. For a perfect gas, ( = specific heat at constant volume),

20 ECMWF Governing Equations 1 Slide 20 Thermodynamic equation (continued) Alternative forms: R=gas constant and Eq. of state:

21 ECMWF Governing Equations 1 Slide 21 Thermodynamic equation (continued) Alternative forms: where The potential temperature is conserved in a Lagrangian dry and adiabatic motion is the potential temperature

22 ECMWF Governing Equations 1 Slide 22 Where do we go from here ? So far : We derived a set of evolution equations based on 3 basic conservation principles valid at the scale of the continuum : continuity equation, momentum equation and thermodynamic equation. What do we want to (re-)solve in models based on these equations? grid scale resolved scale (?) The scale of the grid is much bigger than the scale of the continuum

23 ECMWF Governing Equations 1 Slide 23 Observed spectra of motions in the atmosphere Spectral slope near k -3 for wavelengths >500km. Near k -5/3 for shorter wavelengths. Possible difference in larger-scale dynamics. No spectral gap!

24 ECMWF Governing Equations 1 Slide 24 Scales of atmospheric phenomena Practical averaging scales do not correspond to a physical scale separation. If equations are averaged, there may be strong interactions between resolved and unresolved scales.

25 ECMWF Governing Equations 1 Slide 25 Averaged equations : from the scale of the continuum to the mean grid size scale The equations as used in an operational NWP model represent the evolution of a space-time average of the true solution. The equations become empirical once averaged, we cannot claim we are solving the fundamental equations. Possibly we do not have to use the full form of the exact equations to represent an averaged flow, e.g. hydrostatic approximation OK for large enough averaging scales in the horizontal.

26 ECMWF Governing Equations 1 Slide 26 Averaged equations The sub-grid model represents the effect of the unresolved scales on the averaged flow expressed in terms of the input data which represents an averaged state. The mean effects of the subgrid scales has to be parametrised. The average of the exact solution may *not* look like what we expect, e.g. since vertical motions over land may contain averages of very large local values. The averaging scale does not correspond to a subset of observed phenomena, e.g. gravity waves are partly included at T L 799, but will not be properly represented.

27 ECMWF Governing Equations 1 Slide 27 Demonstration of the averaging effect Use high resolution (10km in horizontal) simulation of flow over Scandinavia Average the results to a scale of 80km Compare with solution of model with 40km and 80km resolution The hope is that, allowing for numerical errors, the solution will be accurate on a scale of 80km Compare low-level flows and vertical velocity cross- section, reasonable agreement Cullen et al. (2000) and references therein

28 ECMWF Governing Equations 1 Slide 28 High resolution numerical solution Test problem is a flow at 10 ms -1 impinging on Scandinavian orography Resolution 10km, 91 levels, level spacing 300m No turbulence model or viscosity, free-slip lower boundary Semi-Lagrangian, semi-implicit integration scheme with 5 minute timestep

29 ECMWF Governing Equations 1 Slide 29 Low-level flow 10km resolution 40km resolution

30 ECMWF Governing Equations 1 Slide 30 Low-level flow 40km resolution 10km resolution averaged to 80km

31 ECMWF Governing Equations 1 Slide 31 Cross-section of potential temperature

32 ECMWF Governing Equations 1 Slide 32 x-z vertical velocity 40km resolution 10km resolution averaged to 80km

33 ECMWF Governing Equations 1 Slide 33 Conclusion Averaged high resolution contains more information than lower resolution runs. The better ratio of comparison was found approximately as dx (averaged high resol) ~ ·dx (lower resol) with ~1.5-2 The idealised integrations suggest that the predictions represent the averaged state well (despite hydrostatic assumption for example). The real solution is much more localised and more intense.


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