Progress towards better representation of observation and ...€¦ · ECMWF Seminar 2014:...

75
Slide 1 Progress towards better representation of observation and background errors in 4DVAR Niels Bormann 1 , Massimo Bonavita 1 , Peter Weston 2 , Cristina Lupu 1 , Carla Cardinali 1 , Tony McNally 1 , Kirsti Salonen 1 1 ECMWF 2 Met Office ECMWF Seminar 2014: Observation and background errors

Transcript of Progress towards better representation of observation and ...€¦ · ECMWF Seminar 2014:...

Page 1: Progress towards better representation of observation and ...€¦ · ECMWF Seminar 2014: Observation and background errors x a Ny (1 N) x b Danger zone: Too small assumed σ o or

Slide 1

Progress towards better representation of

observation and background errors in 4DVAR

Niels Bormann1,

Massimo Bonavita1, Peter Weston2, Cristina Lupu1,

Carla Cardinali1, Tony McNally1, Kirsti Salonen1

1 ECMWF 2Met Office

ECMWF Seminar 2014: Observation and background errors

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Slide 2

Outline

1. Introduction

2. Observation errors

- Overview

- Estimation and specification

- Adjoint methods

3. Background errors

- Introduction

- Hybrid EDA 4DVAR

- Radiance diagnostics

4. Balance of background and observation errors

5. Summary

ECMWF Seminar 2014: Observation and background errors

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Slide 3

Outline

1. Introduction

2. Observation errors

- Overview

- Estimation and specification

- Adjoint methods

3. Background errors

- Introduction

- Hybrid EDA 4DVAR

- Radiance diagnostics

4. Balance of background and observation errors

5. Summary

ECMWF Seminar 2014: Observation and background errors

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Slide 4

Specifying B and R is essential for data assimilation:

- B: Background error covariance: describes random errors in the

background field

- R: Observation error covariance: describes random errors in the

observations and the comparisons observations/model field

Together, they determine the weighting of observations/background.

R and B in the cost function

ECMWF Seminar 2014: Observation and background errors

])[(])[(2

1)()(

2

1)( 11

xHyRxHyxxBxxx T

b

T

bJ

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Slide 5

Optimal weighting:

Consider linear combination

of two estimates xb and y:

22

2

ob

b

Weights given by R and B

Observation weight κ

σo2

σb2

ECMWF Seminar 2014: Observation and background errors

ba xyx )1(

Danger zone: Too small assumed σo or

too large assumed σb can lead to an

analysis worse than the background if

the (true) σo> σb.

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Slide 6

Outline

1. Introduction

2. Observation errors

- Overview

- Estimation and specification

- Adjoint methods

3. Background errors

- Introduction

- Hybrid EDA 4DVAR

- Radiance diagnostics

4. Balance of background and observation errors

5. Summary

ECMWF Seminar 2014: Observation and background errors

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Slide 7

R: Describes random errors in the observations and the comparisons observations/model field.

Systematic errors (biases) are treated separately through bias correction.

Observation error covariance

ECMWF Seminar 2014: Observation and background errors

])[(])[(2

1)()(

2

1)( 11

xHyRxHyxxBxxx T

b

T

bJ

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Slide 8

Contributions to observation error

Measurement error

- E.g., instrument noise for satellite radiances

- Globally constant and uncorrelated if we are lucky.

Forward model (observation operator) error

- E.g., radiative transfer error

- Situation-dependent, likely to be correlated.

Representativeness error

- E.g., point measurement vs model representation

- Situation-dependent, likely to be correlated.

Quality control error

- E.g., error due to the cloud detection scheme missing some

clouds in clear-sky radiance assimilation

- Situation-dependent, likely to be correlated.

ECMWF Seminar 2014: Observation and background errors

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Slide 9

Situation-dependence of observation

error

Examples:

- Cloud/rain-affected radiances: Forward model error and

representativeness error are much larger in cloudy/rainy regions

than in clear-sky regions (see Alan Geer’s talk).

- Effect of height assignment error for Atmospheric Motion Vectors

(see Mary Forsythe’s talk):

ECMWF Seminar 2014: Observation and background errors

Wind

Heig

ht

Low shear – small wind error due to height assignment error

Strong shear – larger wind error due to height assignment error

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Slide 10

Situation-dependence of observation

error

Examples:

- Cloud/rain-affected radiances: Forward model error and

representativeness error are much larger in cloudy/rainy regions

than in clear-sky regions (see Alan Geer’s talk).

- Effect of height assignment error for Atmospheric Motion Vectors

(see Mary Forsythe’s talk):

ECMWF Seminar 2014: Observation and background errors

(Kirsti Salonen)

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Slide 11

Current observation error specification

for satellite data in the ECMWF system

Globally constant, dependent on channel only:

- AMSU-A, MHS, ATMS, HIRS, AIRS, IASI

Globally constant fraction, dependent on impact

parameter:

- GPS-RO

Situation dependent:

- MW imagers: dependent on channel and cloud amount

- AMVs: dependent on level and shear (and satellite, channel,

height assignment method)

Error correlations are neglected.

ECMWF Seminar 2014: Observation and background errors

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Slide 12

Outline

1. Introduction

2. Observation errors

- Overview

- Estimation and specification

- Adjoint methods

3. Background errors

- Introduction

- Hybrid EDA 4DVAR

- Radiance diagnostics

4. Balance of background and observation errors

5. Summary

ECMWF Seminar 2014: Observation and background errors

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Slide 13

How can we estimate R?

Several methods exist, broadly categorised as:

- Error inventory:

Based on considering all contributions to the

error/uncertainty

- Diagnostics with collocated observations, e.g.:

Hollingsworth/Lönnberg on collocated observations

Triple-collocations

- Diagnostics based on output from DA systems, e.g.:

Hollingsworth/Lönnberg

Desroziers et al 2006

Methods that rely on an explicit estimate of B

- Adjoint-based methods

ECMWF Seminar 2014: Observation and background errors

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Slide 14

Departure-based diagnostics

If observation errors and background errors are uncorrelated then:

Statistics of background departures give an upper bound for the true

observation error.

ECMWF Seminar 2014: Observation and background errors

true

T

truebbCov RHHBxHyxHy ])][(]),[[(

Standard deviations of background departures normalised by assumed

observation error for the ECMWF system:

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Slide 15

Observation error diagnostics:

Hollingsworth/Loennberg method

Based on a large database of pairs of departures.

Basic assumption:

- Background errors are spatially correlated, whereas observation

errors are not.

- This allows to separate the two contributions to the variances of

background departures:

ECMWF Seminar 2014: Observation and background errors

Spatially uncorrelated variance

→ Observation error

Spatially correlated variance

→ Background error

Covariance o

f

O—

B [

K2]

Distance between

observation pairs [km]

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Slide 16

Observation error diagnostics:

Desroziers diagnostic

Basic assumptions:

- Assimilation process can be adequately described through linear

estimation theory.

- Weights used in the assimilation system are consistent with true

observation and background errors.

Then the following relationship can be derived:

with (analysis departure)

(background departure)

(see Desroziers et al. 2005, QJRMS)

Consistency diagnostic for the specification of R.

ECMWF Seminar 2014: Observation and background errors

],[~

baCov ddR

])[( aa xHyd

])[( bb xHyd

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Slide 17

Examples of observation error

diagnostics: AMSU-A

ECMWF Seminar 2014: Observation and background errors

Diagnostics for σO, for NOAA-18

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Slide 18

Example: AMSU-A

After thinning to 120 km, error diagnostics suggest little correlations…

ECMWF Seminar 2014: Observation and background errors

Inter-channel error correlations:

Spatial error correlations

for channel 7:

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Slide 19

Example: AMSU-A

… diagonal R a good approximation.

ECMWF Seminar 2014: Observation and background errors

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Slide 20

Example: AMSU-A

… diagonal R a good approximation.

ECMWF Seminar 2014: Observation and background errors

κ

σo2

σb2

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Slide 21

ECMWF Seminar 2014: Observation and background errors

Diagnostics for σO

Examples of observation error

diagnostics: IASI

Temperature sounding LW

WindowWVOzone

Wavenumber [cm-1]

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Slide 22

Example:

IASI

ECMWF Seminar 2014: Observation and background errors

Inter-channel error

correlations

(Hollingsworth/

Lönnberg):

(Updated from Bormann et al 2010)

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Slide 23

Example:

IASI

ECMWF Seminar 2014: Observation and background errors

Inter-channel error

correlations

(Hollingsworth/

Lönnberg):

Humidity

Ozone

Window channels

(Updated from Bormann et al 2010)

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Slide 24

Role of error inflation and error correlation

Experiments:

- Denial: No AIRS and IASI.

- Control: Operational (diagonal) observation errors for AIRS and IASI.

- Diag: Series of experiments with diagonal observation errors for AIRS

and IASI, with σO from HL diagnostic, scaled by a constant factor α:

σO = α σO, HL, with a series of different α

- Cor: Series of experiments with full diagnosed observation error

covariances for AIRS and IASI, again scaled by a factor α:

R = α2 RHL, with a series of different α

Setup:

- 4DVAR, T319 (~60km) resolution, 15 Dec 2011 – 14 Jan 2012

Accounting for inter-channel observation error correlations in the ECMWF system

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Slide 25

ECMWF Seminar 2014: Observation and background errors

Worse

than

Denial

Better

than

Denial

Significant improvement for humidity for experiments with error correlations.

Role of error inflation and error correlation:

Impact on mid-tropospheric humidity

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Slide 26

ECMWF Seminar 2014: Observation and background errors

Worse

than

Denial

Better

than

Denial

For tropospheric temperature, benefit over operations is less clear.

Role of error inflation and error correlation:

Impact on upper tropospheric temperature

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Slide 27

Benefits of taking inter-channel error

correlations into account

Benefits have been found from

taking inter-channel error

correlations into account.

- Some adjustments to diagnosed

matrices needed/beneficial:

Scaling of σO (ECMWF)

Reconditioning (Met Office)

ECMWF Seminar 2014: Observation and background errors

(Peter Weston, Met Office)

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© Crown copyright Met Office

Trial results at Met Office

Verification v Observations Verification v Analyses

+0.209/0.302% UKMO NWP Index +0.241/0.047% UKMO NWP Index

The use of correlated observation errors for IASI was implemented operationally at the Met Office in January 2013

(Peter Weston, Met Office)

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Slide 29

Outline

1. Introduction

2. Observation errors

- Overview

- Estimation and specification

- Adjoint methods

3. Background errors

- Introduction

- Hybrid EDA 4DVAR

- Radiance diagnostics

4. Balance of background and observation errors

5. Summary

ECMWF Seminar 2014: Observation and background errors

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Slide 30

Reduction of assigned

error beneficial

Adjoint diagnostics for observation

errors

Adjoint diagnostics can be used to assess the sensitivity of forecast error reduction to the observation error specification (e.g., Daescu and Todling 2010).

Example: Assessment of IASI in a depleted observing system with only conventional and IASI data.

ECMWF Seminar 2014: Observation and background errors

Increase of assigned

error beneficial (Cristina Lupu, Carla Cardinali)

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Slide 31

Adjoint diagnostics for observation

errors

Adjoint diagnostics can be used to assess the sensitivity of forecast error reduction to the observation error specification.

Example: Assessment of IASI in a depleted observing system with only conventional and IASI data.

ECMWF Seminar 2014: Observation and background errors

Adjoint-based forecast sensitivity to R:Stdev of o-b, normalised by assumed R:

(Cristina Lupu, Carla Cardinali)

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Slide 32

Adjoint diagnostics for observation

errors

Forecast impact from using

observation error reduced to

Desroziers values for selected

33 channels (no error

correlations) in depleted

observing system:

ECMWF Seminar 2014: Observation and background errors

Further work required regarding the applicability of this diagnostic

(consistency of results with estimates of true observation errors).

(Cristina Lupu)

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Slide 33

Summary for observation errors

The representation of observation errors in current data

assimilation systems is mostly fairly basic.

- Common practice is to use globally constant, inflated errors

without error correlations.

- Representation of forward model error, representativeness error

or quality control error is mostly rather crude.

- Benefits are being seen from introducing a more sophisticated

representation of these errors for some data (e.g., situation-

dependence, inter-channel error correlations).

- Efforts to take into account spatial observation error correlations

are very limited.

- Specification of error correlations is likely to be important to

optimise the use of humidity channels and low-noise instruments

(CrIS).

ECMWF Seminar 2014: Observation and background errors

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Slide 34

Observation error correlation

diagnostics for CrIS on S-NPP

ECMWF Seminar 2014: Observation and background errors

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Slide 35

Outline

1. Introduction

2. Observation errors

- Overview

- Estimation and specification

- Adjoint methods

3. Background errors

- Introduction

- Hybrid EDA 4DVAR

- Radiance diagnostics

4. Balance of background and observation errors

5. Summary

ECMWF Seminar 2014: Observation and background errors

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Slide 36

B: Describes random errors in the background fields

Prescribes the structure of the analysis increments

Crucial for carrying forward information from previous observations

Background error covariance

ECMWF Seminar 2014: Observation and background errors

])[(])[(2

1)()(

2

1)( 11

xHyRxHyxxBxxx T

b

T

bJ

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Slide 37

Development of B-modelling within

4DVAR at ECMWF

January 2003, 25r3: Static B generated from an ensemble of data

assimilations (EDA)

April 2005, 29r1: Wavelet B

June 2005, 29r2: Static B from an updated EDA

May 2011, 37r2: Use of flow-dependent background error variances

from an EDA for vorticity

June 2013, 38r2: Use of flow-dependent background error variances

from an EDA for unbalanced control variables

November 2013, 40r1: Flow-dependent background error correlations

from the EDA

ECMWF Seminar 2014: Observation and background errors

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Slide 38• E.g.,: 25 members of 4DVARs • Perturbations from observations, SST, model parameterisations• Provides an estimate of the analysis and background uncertainty.

Ensemble of data assimilations (EDA)

ECMWF Seminar 2014: Observation and background errors

(Fisher 2003)

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Slide 39

Outline

1. Introduction

2. Observation errors

- Overview

- Estimation and specification

- Adjoint methods

3. Background errors

- Introduction

- Hybrid EDA 4DVAR

- Radiance diagnostics

4. Balance of background and observation errors

5. Summary

ECMWF Seminar 2014: Observation and background errors

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Slide 40

At ECMWF, the modelled B has this form:

B = L Σb1/2 C Σb

1/2 LT

L: Balance operator => cross-covariances (mainly mass-wind

balance)

Σb1/2: Standard deviation of BG errors in grid point space

C: Correlation structures of BG errors (wavelet JB, Fisher 2003)

Σb1/2C Σb

1/2: univariate covariances of control variables

Hybrid EDA 4DVAR

Hybrid EDA 4DVAR: Make Σb1/2 and C flow-dependent.

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Slide 41

EDA StDev of LNSP EDA Lscale of BG errors LNSP

ECMWF Seminar 2014: Observation and background errors

Flow-dependent background errors from

the EDA

(Massimo Bonavita)

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Slide 42

Vertical Error Correlation: Vorticity, 850 hPa

Temperature profile

2012/02/10 00Z - (30N, 140W)

(Massimo Bonavita)

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Slide 43

Impact of flow-dependent JB vs static

Normalised reduction in 500 hPa Geopotential RMSE, with 95% confidence, June/July 2012

ECMWF Seminar 2014: Observation and background errors

NH SH

(Massimo Bonavita)

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Slide 44

Example: Hurricane Sandy

ECMWF Seminar 2014: Observation and background errors

Mslp Analysis

30/10/2012 00UTC

Mslp t+204h Fcst valid at

30/10/2012 00UTC

Operational ECMWF forecast provided accurate guidance on landfall position

around a week in advance.

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Slide 45

Hurricane Sandy

Influence of satellite data and EDA

ECMWF Seminar 2014: Observation and background errors

(McNally et al 2014, MWR)

Observed track:

• What happens if we withhold all satellite

observations from polar-orbiters (i.e.,

approx. 90% of obs. counts)?

Track forecast

from

25 Oct 2012

00UTC

Track forecast

from

26 Oct 2012

00UTC

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Slide 46

Hurricane Sandy

Influence of satellite data and EDA

ECMWF Seminar 2014: Observation and background errors

(McNally et al 2014, MWR)

Observed track:

Track forecast

from

25 Oct 2012

00UTC

Track forecast

from

26 Oct 2012

00UTC

Operational forecast

Forecast without polar orbiters and errors

from operational EDA

Forecast without polar orbiter data in EDA

and 4DVAR

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Slide 47

Hurricane Sandy

Influence of satellite data and EDA

ECMWF Seminar 2014: Observation and background errors

(McNally et al 2014, MWR)

Observed track:

Track forecast

from

25 Oct 2012

00UTC

Track forecast

from

26 Oct 2012

00UTC

Operational forecast

Forecast without polar orbiters and

background errors from operational EDA

Forecast without polar orbiter data in EDA

and 4DVAR

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Slide 48

Hurricane Sandy

Influence of satellite data and EDA

ECMWF Seminar 2014: Observation and background errors

(McNally et al 2014, MWR)

Observed track:

Track forecast

from

25 Oct 2012

00UTC

Track forecast

from

26 Oct 2012

00UTC

Operational forecast

Forecast without polar orbiters and

background errors from operational EDA

Forecast without polar orbiter data in EDA

and 4DVAR

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Slide 49

Outline

1. Introduction

2. Observation errors

- Overview

- Estimation and specification

- Adjoint methods

3. Background errors

- Introduction

- Hybrid EDA 4DVAR

- Radiance diagnostics

4. Balance of background and observation errors

5. Summary

ECMWF Seminar 2014: Observation and background errors

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Slide 50

EDA spread in radiance space:

AMSU-A channel 8

ECMWF Seminar 2014: Observation and background errors

15 February 2012, 9 Z

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Slide 51

Skill of the EDA vs observation departures

ECMWF Seminar 2014: Observation and background errors

AMSU-A channel 8 AMSU-A channel 12

February 2012

Calibration required for EDA spread.

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Slide 52

Evolution in assimilation window

Conventional sounders, SAT-section pre-SAC 2013

Example: AMSU-A, channel 8 (100-300 hPa), N. Hem.

Var(Obs – FG)

EDA variance

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Slide 53

Background error estimates in radiance

space [K]

ECMWF Seminar 2014: Observation and background errors

AMSU-A

channel 8

(NeΔT ≈ 0.2 K)

AMSU-A

channel 12

(NeΔT ≈ 0.3 K)

15 February 2012, 9 Z

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Slide 54

Outline

1. Introduction

2. Observation errors

- Overview

- Estimation and specification

- Adjoint methods

3. Background errors

- Introduction

- Hybrid EDA 4DVAR

- Radiance diagnostics

4. Balance of background and observation errors

5. Summary

ECMWF Seminar 2014: Observation and background errors

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Slide 55

Observation/background influence

A measure of the observation influence on the analysis is:

ECMWF Seminar 2014: Observation and background errors

Ta )(])[(

HKy

xHS

1)( RHBHBHKTT

With the Kalman gain

0

5

10

15

20

Cycle 37R2 Cycle 38R2 Cycle 40R1

Total observation influence [%]

(Carla Cardinali)

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Slide 56

Outline

1. Introduction

2. Observation errors

- Overview

- Estimation and specification

- Adjoint methods

3. Background errors

- Introduction

- Hybrid EDA 4DVAR

- Radiance diagnostics

4. Balance of background and observation errors

5. Summary

ECMWF Seminar 2014: Observation and background errors

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Slide 57

Summary/conclusions

Observation errors for satellite data:- Current specifications are mostly fairly basic; errors are mostly

inflated.

- A range of diagnostic tools are available, and these are being

applied to:

Estimate and specify the size of observation errors,

including situation-dependence

Test for error correlations

Specify inter-channel observation error correlations

- Benefits are being obtained from accounting for inter-channel

error correlations and situation-dependent observation errors for

certain data.

Background errors:- Ensemble methods are increasingly used to provide better, flow-

dependent background error statistics.

- This is resulting in significant gains in forecast accuracy.

ECMWF Seminar 2014: Observation and background errors

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Slide 58

Some future perspectives

There is a lot of potential for improved representation of

observation errors in data assimilation systems.

Better understanding of the contributions to observation

error:

- Different treatment for different aspects?

- Interaction between correlated errors and bias correction

- Possibilities to reduce or simplify errors?

- Limitations of diagnostics

Improved representation of background errors as

described by the EDA:

- Enhanced control variables (e.g., clouds, trace gases)

- Refinements to EDA, e.g. in terms of applied perturbations (model

and observations)

ECMWF Seminar 2014: Observation and background errors

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Slide 59

ECMWF Seminar 2014: Observation and background errors

Backup

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Slide 60

Observation error diagnostics:

Hollingsworth/Loennberg method (II)

Drawback: Not reliable when observation errors are

spatially correlated.

ECMWF Seminar 2014: Observation and background errors

Similar methods have been used

with differences between two

sets of collocated observations:

- Example: AMVs collocated with

radiosondes (Bormann et al 2003).

Radiosonde error assumed

spatially uncorrelated.

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Slide 61

Observation error diagnostics:

Desroziers diagnostic (II)

Simulations in toy-assimilation systems:

- Good convergence if the correlation length-scales for

observation errors and background errors are sufficiently

different.

- Mis-leading results if correlation length-scales for background

and observation errors are too similar.

For real assimilation systems, the applicability of the

diagnostic for estimating observation errors is still

subject of research.

ECMWF Seminar 2014: Observation and background errors

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Slide 62

Iterative application of Desroziers

diagnostic

Idealized case: analysis on an equatorial circle (40 000km) with

401 observations/grid-points.

σO, true= 4; Lb = 300 km / L0= 0 km.

σO

σO~

ECMWF Seminar 2014: Observation and background errors

(Desroziers et al 2010)

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Slide 63

σO

σO~

Idealized case: analysis on an equatorial circle (40 000km) with

401 observations/grid-points.

σO, true= 4; Lb = 300 km / L0= 200 km.

Iterative application of Desroziers

diagnostic

ECMWF Seminar 2014: Observation and background errors

(Desroziers et al 2010)

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Slide 64

Example:

IASI

ECMWF Seminar 2014: Observation and background errors

Inter-channel error

correlations

(Hollingsworth/

Lönnberg):

Bormann et al (2010)

Apodisation

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Slide 65

JO-statistics per channel: IASI

ECMWF Seminar 2014: Observation and background errors

Wavenumber [cm-1]Wavenumber [cm-1]

Current obs errors New obs errors

15 July – 4 August 2013

Based on effective departure: deff = (y – H(x))T R-½

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Slide 66

JO-statistics per channel: AIRS

ECMWF Seminar 2014: Observation and background errors

Wavenumber [cm-1]Wavenumber [cm-1]

Current obs errors New obs errors

15 July – 4 August 2013

Based on effective departure: deff = (y – H(x))T R-½

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© Crown copyright Met Office

Reconditioning

(shrinkage)

• Using reconditioned matrix results

in:

• Reduced weight given to IASI obs

• Good convergence

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Slide 68

Trial results from ECMWF

ECMWF Seminar 2014: Observation and background errors

Better background fit to other observations over the tropics, especially for

humidity-sensitive observations:

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Slide 69

Diagnosing Background Error Statistics

Three approaches to estimating Jb statistics:

1. The Hollingsworth and Lönnberg (1986) method

- Differences between observations and the background are a combination of background and observation error.

- Assume that the observation errors are spatially uncorrelated.

2. The NMC method (Parrish and Derber, 1992)

- Assume that the spatial correlations of background error are similar to the correlations of differences between 48h and 24h forecasts verifying at the same time.

3. The Ensemble method (Fisher, 2003)

- Run the analysis system several times for the same period with randomly-perturbed observations and other perturbations.

- Differences between background fields for different runs provide a surrogate for a sample of background error.

ECMWF Seminar 2014: Observation and background errors

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Slide 70

ECMWF Seminar 2014: Observation and background errors

Flow-dependent background errors from

the EDA

2012-01-10 00Z 2012-02-10 00Z

(Massimo Bonavita)

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Slide 71

ECMWF Seminar 2014: Observation and background errors

Flow-dependent background errors from

the EDA

(Massimo Bonavita)

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Slide 72

Massimo Bonavita – DA Training Course 2014 - EDA

Impact of online JBReduction in Geopotential RMSE - 95% confidence

NH SH

50 hPa

100 hPa

200 hPa

500 hPa

1000 hPa

Period: Feb - June 2012

T511L91, 3 Outer Loops (T159/T255/T255)

Verified against operational analysis

(Massimo Bonavita)

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Slide 73

Impact of flow-dependent correlations

Reduction in Geopotential RMSE, including 95% confidence, Feb-June 2012

ECMWF Seminar 2014: Observation and background errors

NH SH

100 hPa

500 hPa

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Slide 74

Calibration factors for AMSU-A

observations

ECMWF Seminar 2014: Observation and background errors

February 2012

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Slide 75

Influence per observation

by observation type

ECMWF Seminar 2014: Observation and background errors

0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1

SYNOPAIREPDRIBUTEMPDROPPILOT

PROFILERGOES-AMV

MTSAT-AMVMeteosat-AMV

MODIS-AMVNOAA-AVHHR

ASCAT-AASCAT-B

OSCATHIRS

AMSU-AATMSAIRSIASI

GPS-ROMERIS

MHSAMSU-B

Meteosat-RadMTSAT-RadGOES-Rad

O3GBRAD

ALLSKY-SSMISALLSKY-TMI

OI

38r2 40R1

(Carla Cardinali)