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Data assimilation: 3DVAR, 4DVAR, and ensemble filters — Examples

1 · Prerequisites

2 · Summary

The examples compute a scalar Gaussian 3DVAR analysis, exhibit a finite-ensemble covariance fluctuation, show a nonlinear-observation case where an EnKF update misses posterior spread, and verify that a strong-constraint 4DVAR objective can have two local minima. Each calculation is tied to its stated covariance, observation, and ensemble assumptions.

3 · Logical flowchart

4 · Definitions, theorems and proofs

None yet.

5 · Examples, counterexamples and false statements

ExampleConstruction: AI-generatedVerification: AI-generatedprecheck passjudge pass (gpt-6-luna)Open item page →

A two-member Gaussian ensemble has a fluctuating covariance

Example

Let X1,X2 be independent N(0,1) forecast members. The divisor-N sample covariance used by Perturbed-observation ensemble Kalman filter at N=2 is random and differs from the true forecast variance with positive probability.

Facts & Assumptions

Given: Independent X1,X2∼N(0,1) and the divisor-N covariance convention of Perturbed-observation ensemble Kalman filter.

[A1]

AC is assumed in the standard-normal construction. The Axiom of Choice

[F1]

The standard normal has density (2π)−1/2e−x2/2, which is strictly positive on every real interval. Standard normal and normal laws

[F2]

N(0,1) has mean zero and variance one under the specified multivariate-normal convention. Multivariate normal law, including singular covariance

[F3]

The EnKF covariance is N−1∑i(Xi−Xˉ)(Xi−Xˉ)T. Perturbed-observation ensemble Kalman filter

Verification

Given: The hypotheses in the Example.

1.1F3givenalgebra

For N=2, Xˉ=(X1+X2)/2, so X1−Xˉ=(X1−X2)/2 and X2−Xˉ=−(X1−X2)/2. By [F3], C2=12((X1−Xˉ)2+(X2−Xˉ)2)=(X1−X2)24.

2.1A1F1F2givenstep 1.1algebra∎

The event A={−0.1<X1<0.1, 3<X2<3.1} has positive probability: each interval has positive probability by [F1], and the variables are independent. On A, X2−X1>2.9, so step 1.1 gives C2>2.92/4=2.1025>1. The true variance of N(0,1) is 1 by [F2]; hence the finite-ensemble covariance differs from it with positive probability.

ExampleConstruction: AI-generatedVerification: AI-generatedprecheck passjudge pass (gpt-6-luna)Open item page →

A strong-constraint 4DVAR objective can have two local minima

Example

Take a one-step strong-constraint window with scalar model map Ψ(u)=u, scalar observation map G(u)=u2, prior mean mb=0, prior covariance B=1, datum y1=1, and observation covariance Γ1=1. The objective in Strong- and weak-constraint 4DVAR with a finite gradient run has two distinct local minima.

Facts & Assumptions

Given: The scalar strong-constraint 4DVAR data in the Example.

[F1]

Strong-constraint 4DVAR minimizes the prior penalty plus observation-misfit penalties along the model trajectory. Strong- and weak-constraint 4DVAR with a finite gradient run

Verification

Given: The objects and parameters in the Example.

1.1F1givenalgebra

Since u1=Ψ(u0)=u0, the one-variable objective from [F1] is J(u)=12u2+12(1−u2)2=12−12u2+12u4.

2.1givenstep 1.1algebra∎

Differentiating gives J′(u)=u(2u2−1). Its only stationary points are 0 and ±1/2. The derivative changes from negative to positive at each of ±1/2, so both are strict local minima. The objective is even, J(±1/2)=3/8<J(0)=1/2, and J(u)→∞ as ∣u∣→∞. Every global minimum is therefore attained at a stationary point, and these two distinct points are both global minimizers. Thus the minimizer is not unique, so an iterative routine's finite definition gives no guarantee that it returns a designated unique solution.

ExampleConstruction: AI-generatedVerification: AI-generatedprecheck passjudge pass (gpt-6-luna)Open item page →

A nonlinear observation makes a symmetric two-member EnKF miss posterior spread

Example

Let the scalar prior be X∼N(0,1) and observe Y=X2+ϵ with independent ϵ∼N(0,γ), γ>0, at datum y=0. Use the finite EnKF forecast ensemble x1=−1,x2=1, identity forecast, and observation map G(x)=x2. The perturbed-observation EnKF update leaves this ensemble unchanged, while the exact posterior has variance strictly below 1.

Facts & Assumptions

Given: AC, the scalar Gaussian prior and error model, y=0, and the forecast ensemble and observation map in the Example.

[A1]

AC is assumed for the Gaussian law construction and density results. The Axiom of Choice

[F1]

The standard normal law has the strictly positive density (2π)−1/2e−x2/2. Standard normal and normal laws

[F2]

N(0,1) has mean zero and variance one. Multivariate normal law, including singular covariance

[F3]

A nondegenerate multivariate normal has the Gaussian Lebesgue density. A positive-definite multivariate normal law has its Gaussian density

[F4]

Bayes' formula gives the posterior density proportional to prior density times likelihood when the marginal density is finite and positive. Bayes formula for dominated kernels

[F5]

The EnKF gain uses the empirical state/observation cross-covariance and each member is updated by its own perturbed observation. Perturbed-observation ensemble Kalman filter

Verification

Given: The hypotheses in the Example.

1.1F5givenalgebra

The predicted observations of both ensemble members equal 1, so their empirical observation variance is 0. Their empirical state-observation cross-covariance is also 0, because the observation deviations are both zero. By [F5] and γ>0, the gain is zero; the update is therefore xa,1=−1, xa,2=1 for every perturbation realization. The updated empirical variance remains 1.

2.1A1F1F2F3F4givenstep 1.1algebra∎

By [A1], [F1], and [F3], the prior and Gaussian likelihood have densities. The likelihood is positive and bounded, so its prior integral is finite and positive; Bayes' formula [F4] makes the posterior density proportional to the even function e−x2/2w(x2), where w(t)=e−t2/(2γ). The posterior mean is therefore zero by symmetry. Put T=X2. Since ET=1 by [F2], E[(T−1)w(T)]=E[(T−1)(w(T)−w(1))]<0. The equality uses E(T−1)=0. The inequality holds because w is strictly decreasing on [0,∞), so the integrand is negative whenever T≠1; the standard normal density gives P(T=1)=0. The integrand is integrable since 0<w≤1 and ET<∞. Thus the posterior variance is Var⁡(X∣Y=0)=E[Tw(T)]E[w(T)]<1. The finite EnKF ensemble variance from step 1.1 is 1, so this admissible nonlinear finite-ensemble update does not equal the exact posterior law.

ExampleConstruction: AI-generatedVerification: AI-generatedprecheck passOpen item page →

Scalar Gaussian 3DVAR returns the exact analysis mean

Example

Take a scalar Gaussian forecast with mean mf=0 and variance B=1, observation map H=1, error variance Γ=1, and observed value y=2. The 3DVAR objective is J(u)=12u2+12(2−u)2.

Facts & Assumptions

Given: AC and the one-dimensional Gaussian prior/error model, with B=Γ=H=1 and y=2.

[A1]

AC is assumed for the Gaussian laws and conditional-law results. The Axiom of Choice

[F1]

The one-step linear-Gaussian model uses independent Gaussian initial and observation errors. Linear-Gaussian state-space models with independent noises

[F2]

The 3DVAR gain is K=BHT(HBHT+Γ)−1 and its analysis is mf+K(y−Hmf). Finite-dimensional 3DVAR analysis

[F3]

The 3DVAR objective minimizer is the Gaussian MAP point and coincides with the Kalman analysis mean under these hypotheses. The 3DVAR quadratic has the Gaussian MAP and Kalman analysis update

[F4]

The exact Kalman analysis covariance is Pa=Pf−KSKT when the innovation S is positive definite. Exact linear-Gaussian Kalman filter

[F5]

Under AC the Kalman recursion is the exact Gaussian conditional law. The finite-horizon linear-Gaussian Kalman filter is exact

Verification

Given: The objects and observations in the Example.

1.1F2givenalgebra

Here S=HBHT+Γ=2 and K=BHTS−1=1/2. Thus the analysis is ma=0+(1/2)(2−0)=1.

2.1A1F1F3F4F5givenstep 1.1algebra∎

The independent Gaussian prior and observation-error model in the Example is the one-step model specified by [F1]. Completing the square gives J(u)=12u2+12(2−u)2=(u−1)2+1, so its unique minimizer is 1, agreeing with step 1.1 and [F3]. The Kalman covariance is Pa=1−(1/2)2(1/2)=1/2 by [F4]; [F5] therefore identifies the exact conditional law as N(1,1/2). The 3DVAR output is its MAP point and supplies no covariance output.

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