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ECMWF Governing Equations 4 Slide 1 Governing Equations IV s to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)
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ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

Mar 29, 2015

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Page 1: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 1

Governing Equations IV

Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold

by Nils Wedi (room 007; ext. 2657)

Page 2: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 2

Introduction and motivation

How do we treat artificial and/or natural boundaries and how do these influence the solution ?

Highlight issues with respect to upper and lower boundary conditions.

Inspire a different thinking with respect to boundaries, which are an integral part of the equations and their respective solution.

Demonstrate the impact of small-scale (or even unresolved) “noise” on the large- scale atmospheric circulation.

Page 3: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 3

Observations of boundary layers: the tropical thermocline

M. Balmaseda

Page 4: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 4

Observations of boundary layers: EPIC - PBL over oceans

M. Koehler

Page 5: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 5

Boundaries

We are used to assuming a particular boundary that fits the

analytical or numerical framework but not necessarily physical free surface, non-reflecting boundary, etc.

Often the chosen numerical framework (and in particular the

choice of the vertical coordinate in global models) favours a

particular boundary condition where its influence on the solution

remains unclear.

Horizontal boundaries in limited-area models often cause

excessive rainfall at the edges and are an ongoing subject of

research (often some form of gradual nesting of different model

resolutions applied).

Page 6: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 6

Choice of vertical coordinate

Ocean modellers claim that only isopycnic/isentropic frameworks maintain dynamic structures over many (life-)cycles ? … Because coordinates are not subject to truncation errors in ordinary frameworks.

There is a believe that terrain following coordinate transformations are problematic in higher resolution due to apparent effects of error spreading into regions far away from the boundary in particular PV distortion. However, in most cases problems could be traced back to implementation issues which are more demanding and possibly less robust to alterations.

Note, that in higher resolutions the PV concept may loose some of its virtues since the fields are not smooth anymore, and isentropes steepen and overturn.

Page 7: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 7

Choice of vertical coordinate

Hybridization or layering to exploit the strength of various coordinates in different regions (in particular boundary regions) of the model domain

Unstructured meshes: CFD applications typically model only simple fluids in complex geometry, in contrast atmospheric flows are complicated fluid flows in relatively simple geometry (eg. gravity wave breaking at high altitude, trapped waves, shear flows etc.)

Bacon et al. (2000)

Page 8: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 8

But why making the equations more difficult ?

Choice 1: Use relatively simple equations with difficult boundaries or

Choice 2: Use complicated equations with simple boundaries

The latter exploits the beauty of

“A metric structure determined by data”Freudenthal, Dictionary of Scientific Biography (Riemann),C.C. Gillispie, Scribner & Sons New York (1970-1980)

Page 9: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 9

Examples of vertical boundary simplifications

Radiative boundaries can also be difficult to implement, simple is perhaps relative

Absorbing layers are easy to implement but their effect has to be evaluated/tuned for each problem at hand

For some choices of prognostic variables (such as in the nonhydrostatic version of IFS) there are particular difficulties with ‘absorbing layers’

Page 10: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 10

Radiative Boundary Conditions for limited height models

eg. Klemp and Durran (1983); Bougeault (1983); Givoli

(1991); Herzog (1995); Durran (1999)

Linearized BoussinesqEquations in x-z plane

Page 11: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 11

Radiative Boundary Conditions

Inserting…

Phase speed:

Group velocity:

for hydrostatic waves

Dispersion relation:

Page 12: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 12

Radiative Boundary Conditions

discretized Fourierseries coefficients:

Page 13: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 13

Wave-absorbing layers eg. Durran (1999)

Viscous damping:

Rayleigh damping:

Adding r.h.s. terms of the form …

Note, that a similar term in the thermodynamic equationmimics radiative damping and is also called Newtonian cooling.

Page 14: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 14

Flow past Scandinavia 60h forecast 17/03/1998 horizontal divergence patterns in the operational configuration

Page 15: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 15

Flow past Scandinavia 60h forecast 17/03/1998horizontal divergence patterns with no absorbers aloft

Page 16: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 16

Wave-absorbing layers: an engineering problem

Page 17: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 17

Wave-absorbing layers: overlapping absorber regions

Finite difference example of an implicit absorber treatment including overlapping regions

Page 18: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 18

The second choice …

Observational evidence of time-dependent well-marked surfaces,

characterized by strong vertical gradients, ‘interfacing’ stratified

flows with well-mixed layers

Can we use the knowledge of the time evolution of the interface ?

Page 19: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 19

Anelastic approximation

Page 20: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 20

Generalized coordinate equations

Strong conservation formulation !

Page 21: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 21

Explanations …

Using:

Solenoidal velocity

Contravariant velocity

Transformation coefficients

Jacobian of the transformation

Physical velocity

Page 22: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 22

Time-dependent curvilinear boundaries

Extending Gal-Chen and Somerville terrain-following coordinate transformation on time-dependent curvilinear boundaries Wedi and Smolarkiewicz (2004)

Page 23: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 23

The generalized time-dependent coordinate transformation

Page 24: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 24

Gravity waves

Page 25: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 25

Reduced domain simulation

Page 26: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 26

Swinging membrane

Swinging membranes bounding a homogeneous Boussinesq fluid

Animation:

Page 27: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 27

Another practical example

Incorporate an approximate free-surface boundary into non-hydrostatic ocean models

“Single layer” simulation with an auxiliary boundary model given by the solution of the shallow water equations

Comparison to a “two-layer” simulation with density discontinuity 1/1000

Page 28: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 28

Regime diagram

supercritical

subcriticalcritical, stationary lee jump

Critical, downstream propagating lee jump

Page 29: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 29

Critical – “two-layer”

Page 30: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 30

Critical – reduced domain

flat

shallow water

Page 31: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 31

Numerical modelling of the quasi-biennial oscillation (QBO) analogue

An example of a zonal mean zonal flow entirely driven by the oscillation of a boundary!

Page 32: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 32

The laboratory experiment of Plumb and McEwanThe principal mechanism of the QBO was demonstrated in the

laboratory

University of Kyoto

Plumb and McEwan, J. Atmos. Sci. 35 1827-1839 (1978)

http://www.gfd-dennou.org/library/gfd_exp/exp_e/index.htm

Animation:

Note: In the laboratory there is onlymolecular viscosity and the diffusivity of salt. In the atmosphere there is also radiative damping.

Page 33: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 33

Time-dependent coordinate transformation

Time dependent boundaries

Wedi and Smolarkiewicz, J. Comput. Phys 193(1) (2004) 1-20

Page 34: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 34

Time – height cross section of the mean flow Uin a 3D simulation

Animation

(Wedi and Smolarkiewicz, J. Atmos. Sci., 2006)

Page 35: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 35

Schematic description of the QBO laboratory analogue

(a) (b)

S = 8

+U

UU

Waves propagating right Waves propagating right

Critical layerprogresses downward

wave interference

filtering filtering

(c) (d)

S = +8

U

+U +U

Waves propagating left Waves propagating left

Critical layerprogresses downward

wave interference

filtering filtering

Page 36: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 36

The stratospheric QBO

- westward+ eastward

(unfiltered) ERA40 data (Uppala et al, 2005)

Page 37: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 37

Stratospheric mean flow oscillations

In the laboratory the gravity waves generated by the oscillating boundary and their interaction are the primary reason for the mean flow oscillation.

In the stratosphere there are numerous gravity wave sources which in concert produce the stratospheric mean flow oscillations such as QBO and SAO (semi-annual oscillation).

Movie courtesy of Glen Shutts

Page 38: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 38

Modelling the QBO in IFS …

Page 39: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 39

Numerically generated forcing!Instantaneous horizontal velocity divergence at ~100hPa

Tiedke massflux scheme

No convection parameterization

T63 L91 IFS simulation over 4 years

Page 40: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 40

Modelling the QBO in IFS ?Not really, due to the lack of vertical resolution to resolve dissipation

processes of gravity waves, possibly also due the lack of appropriate

stratospheric radiative damping, but certainly due to the lack of

sufficient vertically propagating gravity wave sources, which may in

part be from convection, which in itsself is a parameterized process.

A solution is to incorporate (parameterized) sources of (non-

orographic) gravity waves. These parameterization schemes

incorporate the sources, propagation and dissipation of momentum

carried by the gravity waves into the upper atmosphere (typically <

100hPa)

The QBO is perhaps of less importance in NWP but vertically

propagating waves (either artificially generated or resolved) and their

influence on the mean global circulation are very important!

Page 41: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

35r2

SPARC

July climatology

Page 42: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

35r3

SPARC

July climatology

Page 43: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 43

QBO : Hovmöller from free 6y integrations=no nonoro GWD

Difficult to find the right level of tuning !!!

Page 44: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 44

Comparison of observed and parametrized GW momentum flux for 8-14 August 1997 horizontal distributions of absolute values of momentum flux (mPa) Observed values are for CRISTA-2 (Ern et al. 2006). Observations measure temperature fluctuations with infrared spectrometer, momentum fluxes are derived via conversion formula.

Parametrized non-orographic gravity wave momentum flux

Page 45: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 45

A. Orr, P. Bechtold, J. Scinoccia, M. Ern, M. Janiskova (JAS 2009 to be submitted)

Total = resolved + parametrized wave momentum flux

Page 46: ECMWF Governing Equations 4 Slide 1 Governing Equations IV Thanks to Piotr Smolarkiewicz, Glen Shutts and Peter Bechtold by Nils Wedi (room 007; ext. 2657)

ECMWFGoverning Equations 4 Slide 46

Resolved and unresolved gravity waves

The impact of resolved and unresolved gravity waves on the circulation and model bias remains an active area of research.

Note the apparent conflict of designing robust and efficient numerical methods (i.e. implicit methods aiming to artificially reduce the propagation speed of vertically propagating gravity waves or even the filtering of gravity waves such as to allow the use of large time-steps) and the important influence of precisely those gravity waves on the overall circulation. Most likely, the same conflict does not exist with respect to acoustic waves, however, making their a-priori filtering feasible…