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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.

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