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1 ECMWF Seminar on Recent Developments in Atmospheric and Ocean Data Assimilation. Sept 2003. © Crown copyright Relative Merits of 4D-Var and Ensemble Kalman Filter Andrew Lorenc Met Office, Exeter
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Page 1: Relative Merits of 4D-Var and Ensemble Kalman Filter · Sampl ed by ensemble (flow-dependent). Noisy: must be modified to have compact support using Schur product. Ability to fit

1 ECMWF Seminar on Recent Developments in Atmospheric and Ocean Data Assimilation. Sept 2003. © Crown copyright

Relative Merits of 4D-Var and Ensemble Kalman Filter

Andrew LorencMet Office, Exeter

Page 2: Relative Merits of 4D-Var and Ensemble Kalman Filter · Sampl ed by ensemble (flow-dependent). Noisy: must be modified to have compact support using Schur product. Ability to fit

2 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

OutlineConsider 4D-Var & EnKF for NWP applicationsLook at how they represent covariances, and hence

their expected properties

Incremental 4D-Var as a 4D covariance model

EnKF sampling of covariancesCompare assimilation characteristicsEase of implementationTwo ways forward

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3 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Data AssimilationRepresent

– in terms of NWP model variables– Uncertainty ⇒ PDF of all variables

Evolve– using physically based NWP equations– should propagate uncertainty & allow for model

error ⇒ Fokker-Planck equation

Combine using Bayes theorem– characterise observation uncertainties– PDFs are unknowable!

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4 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Data AssimilationRepresent

– in terms of NWP model variables– Uncertainty ⇒ PDF of all variables

Evolve– using physically based NWP equations– should propagate uncertainty & allow for model

error ⇒ Fokker-Planck equation

Combine using Bayes theorem– characterise observation uncertainties– PDFs are unknowable!

Page 5: Relative Merits of 4D-Var and Ensemble Kalman Filter · Sampl ed by ensemble (flow-dependent). Noisy: must be modified to have compact support using Schur product. Ability to fit

5 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Fokker-Planck Equation

pdft0

pdft0

`

chaotic growth + model errorincrease spread

pdft1

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6 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Data AssimilationRepresent

– in terms of NWP model variables– Uncertainty ⇒ PDF of all variables

Evolve– using physically based NWP equations– should propagate uncertainty & allow for model

error ⇒ Fokker-Planck equation

Combine using Bayes theorem– characterise observation uncertainties– PDFs are unknowable!

Page 7: Relative Merits of 4D-Var and Ensemble Kalman Filter · Sampl ed by ensemble (flow-dependent). Noisy: must be modified to have compact support using Schur product. Ability to fit

7 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Bayes’ Theorem

Observationx b2

x 2a

x 1bx 1a

pdff

pdfay o=(x

1 +x2 )/2

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8 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Flaws in “traditional” 4D-Var derivation

The atmosphere can be chaotic at most scales, some with very short timescales.The 4D-Var penalty function for a “perfect” model will be fractal because of the chaotic scales represented, so a descent algorithm cannot work.There is no basis for saying the maximum of a complicated PDF is the best analysis.

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9 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Synoptic-scale Incremental 4D-Var

Assume background PDFs are GaussianReduce dimensionalityLinear evolutionBuilds on existing 3D-VarCan be thought of as a 4D (time & space) PDF describing uncertainty, for use in Bayesian fit to all observations in a 4D time-window.

Page 10: Relative Merits of 4D-Var and Ensemble Kalman Filter · Sampl ed by ensemble (flow-dependent). Noisy: must be modified to have compact support using Schur product. Ability to fit

10 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Incremental 4D-Var

SimplifiedGaussian

pdf t0

` SimplifiedGaussian

pdf t1

Full model evolves mean of pdf

PF model evolves any simplified perturbation,and hence covariance of pdf

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11 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Incremental 4D-Var3D-Var supplies 3D covariance at t=0, consistent with dynamical balance relationshipsPF model evolves this in time, to create a 4D covariance consistent with PF equationsDo a 4D fit to observations in the time-windowCovariances define relative weighting, interpolation and extrapolation of observations in space & timeCovariances (thro’ null-space) define classes of 4D analysis increments which are not allowed

(e.g. unbalanced, or inconsistent with PF equations)

Page 12: Relative Merits of 4D-Var and Ensemble Kalman Filter · Sampl ed by ensemble (flow-dependent). Noisy: must be modified to have compact support using Schur product. Ability to fit

Incremental 4D-Var Equationsδ x is 4D increment to 4D guess: g δ= +x x x

Want 4D fit, minimising:( ) ( ) ( ) ( )

( ) ( )

112

112

Tb b

To o

J δ δ δ δ δ−

= − −

+ − −

xx x x B x x

y y R y y

y is prediction of obs in time window: ( )H=y x

v is transformed control variable: ISδ −=x MUvIS− is incrementing operator,

M is Perturbation Forecast model,U is 3DVAR variable transform,

IS− MU models 4D covariance ( )xB :( )

TI T TS S− −=xB MUU M

Transformed minimisation: ( ) ( ) ( )11 12 2

To oTJ −= + − −v v v y y R y y

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13 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Benefits of 4D-VarRetains benefits of 3D-Var:

– assimilation of radiances, good balance, …

Better than 3D-Var in using obs where there are tendencies represented by PF model

– e.g. baroclinic developments ⇒ severe weather

Scope for better assimilation of cloud and ppn

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14 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Ensemble Kalman Filter

Gaussianpdf t0

` Gaussianpdf t1

Full model evolves each ensemble member

Mean & covariance of ensemble membersdefine evolved pdf

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15 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Extended Kalman Filter

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16 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

EnKF

=

=

=

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17 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

A form of square-root filter:

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18 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Errors in sampled EnKF covariances

N=100

-0.5

0

0.5

1

1.5

0 500 1000 1500 2000 2500 3000

distance (km)

cova

rianc

e

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19 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Errors in sampled EnKF covariances (2)

A sub-optimal Kalman gain calculated using the estimatedcovariances:

( ) 1−+= RHHPHPK Tfe

Tfee ,

gives larger analysis errors, which can be calculated if one knowsthe true covariance:

( ) Te

Tfe

fe

fa KRHHPKHPKPP ++−= 2 .

Global average variance, using a perfect ob:• Correct K gives 1–0.0015• Sampled eK gives 1+0.0087

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20 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

The Schur or Hadamard Product

Curve C chosen such that covariances go to zero at distance. e.g. compactly supported (4.10) from Gapsari and Cohn (1999)

This gives:Ensemble covariances modified to be 0 at distance.Covariance function slightly narrower than ideal.

n=100 * compact support

-0.5

0

0.5

1

1.5

0 500 1000 1500 2000 2500 3000

distance (km)

cova

rianc

e

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21 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Best scale for C depends on ensemble size N:

-0.002

0

0.5 1 1.5 2 2.5 3 3.5 4

relative scale of correlation

chan

ge in

glo

bal e

rror

var

ianc

eN=10N=20N=40N=100N=1000idealbest

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22 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Choices in EnKFTreat pdfs as Gaussian

– represented by mean & covariance– excludes Ens DA methods for small nonlinear problems

Localise covariances– excludes ETKF

How to generate analysis ensemble?? Perturbed observations? Transform methods (ETKF EAKF EnSRF)

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23 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Perturbed model & observation ensemble

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24 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Transform methods avoiding perturbed obsUsing SVD, transform { }fix w ith covariance Tf f f=P X X

into { }aix w ith ( ) 1Ta a a f f T f T f−

= = − +P X X P PH HPH R HP :

1) Update all ensemble by mean increment.2) Scale perturbations to have correct covariance: - Ensemble Adjustment Kalman Filter (Anderson):

a T f=X A X . - Ensemble Transform Kalman Filter (Bishop):

a f=X X T. - Ensemble square root filter (Tippett et al):

sequential processing of obs

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25 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Properties of transform methods

Mathematically equivalent for Gaussian pdfsReduces errors due to noisy estimation of covariances (Whitaker & Hamill)If covariance localisation is wanted, then only practicable with sequential processing of obsLocalised sequential processing EnSRF is simple to code and implement

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26 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Degenerate covariancesThe basic EnKF (without the Schur product) only has N degrees of freedom available to fit the observations.A perfect observation removes a degree of freedom from the ensemble:So the EnKF can only fit N pieces of information (in an area whose size depends on the Schur product correlation scale).

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27 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Degenerate covariances

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28 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Balance

Page 29: Relative Merits of 4D-Var and Ensemble Kalman Filter · Sampl ed by ensemble (flow-dependent). Noisy: must be modified to have compact support using Schur product. Ability to fit

29 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Effect of Schur product on geostrophic balance

Height covariances drop off more steeply,

increasing geostrophic wind inplied by a single height observation,

but height-wind covariances are reduced, reducing actual wind increments.

Effect of Schur product on balance

0.5

0.6

0.7

0.8

0.9

1

10 100 1000

N

sub-

geos

trop

hic

fact

or

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30 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Non-Gaussian Analysis Equations (1)

Can be done in principle, but too difficult & costly for NWP - requires nonlinear ensemble adjustment, orresampling.I only consider applying the standard eqn to:1 non-linear observation operators2 Quality Control

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31 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

-6

-4

-2

0

2

4

6

8

10

12

-6 -4 -2 0 2 4 6 8 10

-6

-4

-2

0

2

4

6

8

10

12

-6 -4 -2 0 2 4 6 8 1

-4

-2

0

2

4

6

8

10

12

-6 -4 -2 0 2 4 6 8 10

-4

-2

0

2

4

6

8

10

12

-6 -4 -2 0 2 4 6 8 10

Forecast (u,v). sd(u)=sd(v)=2. Forecast (u,s)

Analysed (u,v) for s=3, sd(s)=0. Analysed (u,v) for s=3, sd(s)=1.

Example EnKFof a wind speed ob (N=1000).

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32 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Non-Gaussian Analysis Equations (2)Quality Control

For situations where information from nearby observations helps (e.g. extreme obs corroborating each other), Var with a non-quadratic penalty function should do better than the (sequential Gaussian) EnKF.But many QC decisions are in data-sparse areas, where the principle source of corroborative information is the forecast. If the error variance “of the day” from the ensemble, despite sampling noise, is more accurate than that assumed in Var, then the EnKF will do better.

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33 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Assimilation characteristicsIncremental 4D-Var EnKF

Forecastcovariances

Modelled at t0 (usuallyisotropic), time evolution for afinite time-window representedby linear and adjoint models.

Sampled by ensemble (flow-dependent). Noisy: must bemodified to have compactsupport using Schur product.

Ability to fitdetailedobservations.

Limited by resolution ofsimplified model.Tendencies fitted within time-window.

Fewer data (in a region) thanensemble members.Tendency information onlyextracted if obs properly fitted.

Balance constraints Can be imposed through adynamical design to thevariable transform, or a separatebalance penalty.

Only imposed if each forecast inthe ensemble is balanced. Lostslightly in Schur product.

Nonlinearobservationoperators

Allowed if differentiable.(Results uncertain if pdf isbimodal in range of interest.)

Allowed, but resulting pdfmodelled by Gaussian.

Non-Gaussianobservational errors

Allowed if differentiable.(Results uncertain if pdf isbimodal in range of interest.)

Not allowed. Prior QC step isneeded.

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34 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Practical characteristicsIncremental 4D-Var EnKF

Forecastmodel

Predict evolution of mean.No switches.

Predict typical state. May havestochastic physics and switches.

Linearmodel

Predict average evolution of finiteperturbations from the mean.May be simplified.

Not needed.

Adjointmodel

Needed for (simplified) linearmodel.

Not needed.

Covariancemodel

Significant effort for covariancemodel. Adjoint code needed.

Simple correlation in Schurproduct. Covariance inflation tokeep the right spread.

Observationoperators

Linear and adjoint operatorsneeded (not usually difficult).

Only uses forward operators.

Analysisalgorithm

Descent algorithm available as "offthe shelf" software.

EnSRF very easy.Simultaneous box algorithms aremore complicated (like OI).

Suitabilityfor parallelcomputers

Require parallel simplified andadjoint models.

Forecasts can run in parallel.Covariances require a transposition.Sequential proc of obs difficult.

Limited-areamodelling

Error covariance models OK tospecify boundary value errors

Ensemble of global forecasts toprovide boundary conditions.

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35 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Two possible ways forward

Hybrid 4D-Var - EnKF for mainstream NWP

Nested EnKF for special applications

Page 36: Relative Merits of 4D-Var and Ensemble Kalman Filter · Sampl ed by ensemble (flow-dependent). Noisy: must be modified to have compact support using Schur product. Ability to fit

36 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Mainstream NWP Systems - requirementsHigh resolution to reduced errors of representativenessAnalyse all scales with significant errorsQuality control observationsUse nonlinear observationsUpdate satellite bias correctionsBetter (mean) short-period forecast

more important than better error estimates

VAR can address all of these simultaneously⇒Seek to enhance it by adding benefits of EnKF

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37 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Variational use of EnKF covariance (1)

Can use the ensemble generated covariances in a variational algorithmThis should give identical results to the mean from an ideal EnKF algorithmAs usual with VAR, the analysis error covariance is not automatically obtainedSo the VAR method cannot easily generate an ensemble, but it can use one made by another system.

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38 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Variational use of EnKF covariance (1)

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39 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

(2)

Similarly, VAR can

use ensemble

covariances modified by

a Schurproduct:

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40 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

β

(3)

VAR can use the ensemble to augment the “traditional” covariance

model with some Errors Of The

Day.

Dale Barker & Adrian Semple at Met Office.Hamill & Snyder (2000).

Should reduce “traditional” error covariances to compensate for those represented by the ensemble (β>1).

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41 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Response to a single T ob

Basic 3D-Var 3D-Var + 1 bred modeDale Barker EOTD expts.Mark Dubal GCT expts.Adrian Semple, 2001: A Meteorological Assessment of the Geostrophic Co-ordinate Transform and Error Breeding System When used in 3D Variational Data Assimilation. NWP Tech Rep 357.

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42 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

Hybrid 4D-Var EnKF - a possible scenarioHigh resolution “control” NWP model, for the best possible prediction of the “best” estimate.Incremental 4D-Var, using all relevant observations in a time-window (including nonlinear H, and QC).Final outer-iteration at sufficient resolution to extract information from the tendencies between consecutive observed fields.Background Covariances in 4D-Var enhanced by synoptic-scale Errors of The Day from an ensemble of perturbations.Ensemble propagated using an ETKF

centred on the high-res 4D-Var control.

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43 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

EnKF for special applicationsLarge uncertainty ⇒ difficulty with 4D-Var:

– Deterministic NWP model for ensemble mean– Evolution of perturbations nonlinear

EnKF can work with large uncertainty:– Sparse observations (Whitaker et al.)– Idealized convective-scale, with no large-scale errors (Snyder & Zhang)

EnKF is easy to develop, even if model is also developing

Use EnKF for R&D of new NWP applications with large uncertainty (e.g. convective-scale)

Nested in mainstream NWP bcs to give synoptic-scales

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44 Andrew Lorenc. ECMWF Seminar, Sept 2003. © Crown copyright

4D-Var vEnKF

Summary


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