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A comparison of hybrid ensemble transform Kalman filterETKF3DVAR and ensemble square root filter EnS

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Comparison of flow dependent background error covariance models (Hybrid 50 mem. result) ... yo. VAR. Xb. Xa. ETKF. Pb. mean. gen_be. VAR da_ntmax=0. sum. Xf1 ... – PowerPoint PPT presentation

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Title: A comparison of hybrid ensemble transform Kalman filterETKF3DVAR and ensemble square root filter EnS


1
A comparison of hybrid ensemble transform Kalman
filter(ETKF)-3DVAR and ensemble square root
filter (EnSRF) analysis schemes
  • Xuguang Wang
  • NOAA/ESRL/PSD, Boulder, CO
  • Thomas M. Hamill
  • Jeffrey S. Whitaker
  • NOAA/ESRL/PSD, Boulder, CO
  • Craig H. Bishop
  • NRL, Monterey, CA

2
Why hybrid ETKF-3DVAR ?
  • Hybrid ETKF-3DVAR is expected to be less
    expensive than EnSRF, and still can benefit from
    ensemble-estimated error statistics.
  • The hybrid may be more robust for small ensemble
    size, since can adjust the amount of static vs.
    ensemble covariance used.
  • The hybrid can be conveniently adapted to the
    existing variational framework.

3
Hybrid ETKF-3DVAR
member 1 forecast
member 1 analysis
member 1 forecast
ETKF update perturbations
member 2 forecast
member 2 analysis
member 2 forecast
member 3 forecast
member 3 analysis
member 3 forecast
ETKF-3DVAR update mean
data assimilation
forecast
4
Hybrid ETKF-3DVAR updates mean
  • Background error covariance is approximated by a
    linear combination of the sample covariance
    matrix of the ETKF forecast ensemble and the
    static covariance matrix.

  • Can be conveniently adapted into the operational
    3DVAR through augmentation of control variables
    (Lorenc 2003 Buehner 2005 Wang et al. 2006).

5
ETKF updates perturbations
  • ETKF transforms forecast perturbations into
    analysis perturbations by
  • where is chosen by trying to solve the
    Kalman filter error covariance update equation,
    with forecast error covariance approximated by
    ensemble covariance.
  • Latest formula for (Wang et al. 20042006,
    MWR)
  • Computationally inexpensive for ensemble size of
    o(100), since transformation fully in
    perturbation subspace.

6
Experiment design
  • Numerical model
  • Dry 2-layer spectral PE model run at T31
  • Model state consists of vorticity, divergence
    and layer thickness of Exner function
  • Error doubling time is 3.78 days at T31
  • Perfect model assumption

(Hamill and Whitaker MWR, 2005)
  • Observations
  • 362 Interface and surface Exner functions taken
    at equally spaced locations
  • Observation values are T31 truth plus random
    noise drawn from normal distribution
  • Assimilated every 24h

7
Experiment design
  • Update of mean (OI) and formulation of B
  • In this experiment, the hybrid updates the mean
    using

whose solution is equivalent to that if solved
variationally under our experiment design.
  • The static error covariance model is constructed
    iteratively from a large sample of 24h fcst.
    errors.

8
RMS analysis errors 50 member
  • Improved accuracy of EnSRF over 3DVAR can be
    mostly achieved by the hybrid.
  • Covariance localization applied on the ETKF
    ensemble when updating the mean (but not applied
    when updating the perturbations) improved the
    analyses of the hybrid.

9
RMS analysis errors 20 member
  • Both 20mem hybrid and EnSRF worse than 50mem,
    but still better than 3DVAR
  • Hybrid nearly as accurate (KE, ??2 norms) or
    even better (surface ? norm) compared to EnSRF

10
RMS analysis errors 5 member
EnSRF filter divergence
  • EnSRF experienced filter divergence for all
    localization scales tried.
  • Hybrid was still more accurate than the 3DVAR.
  • Hybrid is more robust in the presence of small
    ensemble size.

11
Comparison of flow dependent background error
covariance models
(Hybrid 50 mem. result)
(EnSRF 50 mem. result)
12
Initial-condition balance
  • Analysis is more imbalanced with more severe
    localization.
  • Analyses of the hybrid with the smallest rms
    error are more balanced than those of the EnSRF,
    especially for small ensemble size (not shown).

(50 mem. result)
13
Spread-skill relationships
  • Overall average of the spread is approximately
    equal to overall average of rms error for both
    EnSRF and Hybrid.
  • Abilities to distinguish analyses of different
    error variances are similar for EnSRF and Hybrid.

(20 mem. result)
14
Summary
  • The hybrid analyses achieved similar improved
    accuracy of the EnSRF over 3DVAR.
  • The hybrid was more robust when ensemble size was
    small.
  • The hybrid analyses were more balanced than the
    EnSRF analyses, especially when ensemble size was
    small.
  • The ETKF ensemble variance was as skillful as the
    EnSRF.
  • The hybrid can be conveniently adapted into the
    existing operational 3DVAR framework.
  • The hybrid is expected to be less expensive than
    the EnSRF in operational settings.

15
Preliminary results with resolution model error
  • T127 run as truth imperfect model run at T31
  • 200-member ensembles
  • Additive model error parameterization
  • comparable rms errors for hybrid and EnSRF

16
Hybrid ETKF-3DVAR for WRF(collaborated with Dale
Barker and Chris Snyder)
  • a-control variable method (Lorenc 2003) to
    incorporate ensemble in WRF-VAR

17

Statistics of iteratively constructed B
balance
rms analysis errors
18
Ensemble square-root filter(Whitaker and
Hamill,MWR,2002)
  • Background error covariance is estimated from
    ensemble with covariance localization.
  • Mean state is corrected to new observations,
    weighted by the Kalman gain.
  • Reduced Kalman gain is calculated to update
    ensemble perturbations.
  • Observations are serially processed. So cost
    scales with the number of observations.

obs1
obs2
obs3
EnSRF
EnSRF
EnSRF
  • Covariance localization can produce imbalanced
    initial conditions.

19
Maximal perturbation growth
  • Find linear combination coefficients b to
    maximize
  • Maximal growth in the ETKF ensemble perturbation
    subspace is faster than that in the EnSRF
    ensemble perturbation subspace.
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