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Introduction to Data Assimilation: Lecture 2

Introduction to Data Assimilation: Lecture 2. Saroja Polavarapu Meteorological Research Division Environment Canada. PIMS Summer School, Victoria. July 14-18, 2008. Outline of lecture 2. Covariance modelling – Part 1 Initialization (Filtering of analyses) Basic estimation theory

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Introduction to Data Assimilation: Lecture 2

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  1. Introduction to Data Assimilation: Lecture 2 Saroja Polavarapu Meteorological Research Division Environment Canada PIMS Summer School, Victoria. July 14-18, 2008

  2. Outline of lecture 2 • Covariance modelling – Part 1 • Initialization (Filtering of analyses) • Basic estimation theory • 3D-Variational Assimilation (3Dvar)

  3. Background error covariance matrix filters analysis increments Analysis increments (xa – xb) are a linear combination of columns of B Properties of B determine filtering properties of assimilation scheme!

  4. A simple demonstration of filtering properties of B matrix K

  5. Choose a correlation function and obs increment shape then compute analysis increments cos(x) cos(2x) sobs/sb = 0.5

  6. cos(3x) cos(4x) cos(5x) cos(6x)

  7. cos(7x) cos(9x) cos(8x) cos(10x)

  8. 1. Covariance Modelling • Innovations method • NMC-method • Ensemble method

  9. Background error covariance matrix • If x is 108, Pb is 108 x 108. • With 106 obs, cannot estimate Pb. • Need to model Pb. • The fewer the parameters in the model, • the easier to estimate them, but • less likely the model is to be valid

  10. m j r j q r r r q l i i m 1. Innovations method • Historically used for Optimal Interpolation • (e.g. Hollingsworth and Lonnberg 1986, • Lonnberg and Hollingsworth 1986, Mitchell et al. 1990) • Typical assumptions: • separability of horizontal and vertical correlations • Homogeneity • Isotropy l

  11. Background error Instrument+ representativeness Choose obs s.t. these terms =0 Dec. 15/87-Mar. 15/88 radiosonde data. Model: CMC T59L20 Assume homogeneous, isotropic correlation model. Choose a continuous function r(r) which has only a few parameters such as L, correlation length scale. Plot all innovations as a function of distance only and fit the function to the data. Mitchell et al. (1990)

  12. Obs and Forecast error variances Mitchell et al. (1990) Mitchell et al. (1990)

  13. Vertical correlations of forecast error Height Lonnberg and Hollingsworth (1986) Non-divergent wind Hollingsworth and Lonnberg (1986)

  14. Multivariate correlations Bouttier and Courtier www.ecmwf.int 2002 Mitchell et al. (1990)

  15. If covariances are homogeneous, variances are independent of space Covariances are not homogeneous If correlations are homogeneous, correlation lengths are independent of location Correlations are not homogeneous

  16. Correlations are not isotropic Gustafsson (1981) Daley (1991)

  17. Are correlations separable? If so, correlation length should be Independent of height. Lonnberg and Hollingsworth (1986) Mitchell et al. (1990)

  18. Covariance modelling assumptions: • No correlations between background and obs errors • No horizontal correlation of obs errors • Homogeneous, isotropic horizontal background error correlations • Separability of vertical and horizontal background error correlations None of our assumptions are really correct. Therefore Optimal Interpolation is not optimal so it is often called Statistical Interpolation.

  19. 2. Initialization • Nonlinear Normal Mode (NNMI) • Digital Filter Initialization (DFI) • Filtering of analysis increments

  20. Balance in data assimilation Daley 1991

  21. The “initialization” step • Integrating a model from an analysis leads to motion on fast scales • Mostly evident in surface pressure tendency, divergence and can affect precipitation forecasts • 6-h forecasts are used to quality check obs, so if noisy could lead to rejection of good obs or acceptance of bad obs • Historically, after the analysis step, a separate “initialization” step was done to remove fast motions • In the 1980’s a sophisticated “initialization” scheme based on Normal modes of the model equations was developed and used operationally with OI.

  22. Consider model Determine modes Separate R and G Project onto G Define balance Solution Nonlinear Normal Mode Initialization (NNMI)

  23. G S A N R L The slow manifold

  24. Daley 1991

  25. Digital Filter Initialization (DFI) Lynch and Huang (1992) N=12, Dt=30 min Tc=6 h Tc=8 h Fillion et al. (1995)

  26. Combining Analysis and Initialization steps • Doing an analysis brings you closer to the data. • Doing an initialization moves you farther from the data. Gravity modes N Rossby modes Daley (1986)

  27. Variational Normal model initialization Minimize I such that uI, vI, fI stays on M. Daley (1978), Tribbia (1982), Fillion and Temperton (1989), etc. Daley (1986)

  28. Some signals in the forecast e.g. tides should NOT be destroyed by NNMI! So filter analysis increments only Semi-diurnal mode has amplitude seen in free model run, if anl increments are filtered Seaman et al. (1995)

  29. 3. A bit of Estimation theory(will lead us to 3D-Var)

  30. a posteriori p.d.f.

  31. Data Selection From: ECMWF training course available at www.ecmwf.int Bouttier and Courtier (2002)

  32. The effect of data selection PSAS OI Cohn et al. (1998)

  33. The effect of data selection Cohn et al. (1998)

  34. Advantages of 3D-var • Obs and model variables can be nonlinearly related. • H(X), H, HT need to be calculated for each obs type • No separate inversion of data needed – can directly assimilate radiances • Flexible choice of model variables, e.g. spectral coefficents • No data selection is needed.

  35. 3D-Var Preconditioning (1) • Hessian of cost function is B-1 + HTR-1H • To avoid computing B-1 in (1), change control variable to dx=Lc so first term in (1) becomes ½ ccT and we minimize w.r.t. c. Heredx=x-xb • After change of variable, Hessian is I + term • If no obs, preconditioner is great, but with more obs, or more accurate obs, it loses its advantage

  36. With covariances in spectral space, longer correlation lengths scales are permitted in the stratosphere With flexibility of choice of obs, can assimilate many new types of obs such as scatterometer Andersson et al. (1998) Andersson et al. (1998)

  37. 14 13 12 11 10 9 8 7 6 5 To assimilate radiances directly, H includes an instrument-specific radiative transfer model Normalized AMSU weighting functions

  38. Impact of Direct Assimilation of Radiances • Anomaly = difference between forecast and climatolgy • Anomaly correlation = pattern correlation between forecast anomalies and • verifying analyses 1974 – improved NESDIS VTPR Retrievals 1978 – TOVS retrievals Kalnay et al. (1998)

  39. Operational weather centers used 3D-Var from1990’s *Later replaced by 4D-Var

  40. Summary (Lecture 2) • Estimation theory provides mathematical basis for DA. Optimality principles presume knowledge of error statistics. • For Gaussian errors, 3D-var and OI are equivalent in theory, but different in practice • 3D-var allows easy extension for nonlinearly related obs and model variables. Also allows more flexibility in choice of analysis variables. • 3D-var does not require data selection so analyses are in better balance. • Improvement of 3D-var over OI is not statistically significant for same obs. Systematic improvement of 3DVAR over OI in stratosphere and S. Hemisphere. Scores continue to improve as more obs types are added.

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