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Independent perturbed-observation reference members follow the Kalman filter
Statement
Assume AC and the finite-horizon linear-Gaussian model of Linear-Gaussian state-space models with independent noises, with for . Fix the observation values . For each , initialize iid with the model's prior. At each time use independent per-member noises and , independent across and from the preceding ensemble, and form where is the deterministic gain from Exact linear-Gaussian Kalman filter. Then, for every , the analysis members are iid with law , the exact Kalman filtering law at the fixed data .
Facts & Assumptions
Given: AC, the finite-horizon linear-Gaussian model, , and the independent per-member initialization and perturbations in the Statement.
AC is the axiom required by the multivariate-normal and Kalman suppliers. The Axiom of Choice
The state and observation equations are affine with mutually independent Gaussian initial, process, and observation noises; their covariance matrices may be positive semidefinite. Linear-Gaussian state-space models with independent noises
A finite independent stack of multivariate normal vectors is jointly multivariate normal, including for singular covariance blocks. A finite stack of independent Gaussian vectors is jointly Gaussian
The Kalman algorithm predicts , and updates by , . Exact linear-Gaussian Kalman filter
Under the stated model and positive-definite innovation matrices, these recursions are exact Gaussian conditional laws at every observation history. The finite-horizon linear-Gaussian Kalman filter is exact
A multivariate normal law permits singular positive-semidefinite covariance and is closed under the defining affine projections. Multivariate normal law, including singular covariance
Proof
Given: The hypotheses in the Statement.
At , the analysis members are iid with law by their initialization, so the claim holds at the base time.
Assume the induction hypothesis: the members at time are iid with law . Each forecast is an affine image of the independent Gaussian pair . By [F2] the pair is jointly Gaussian; every scalar projection of its affine image is a scalar Gaussian projection, so [F5] makes the forecasts iid Gaussian with mean and covariance .
Since and , , so is defined. The independent Gaussian pair and [F2] show that , with , is Gaussian. Its mean is and its covariance is because . These are precisely the Kalman update parameters in [F3].
For distinct member indices the pairs of forecast and perturbed observation are independent by the input independence and the induction hypothesis; applying the same deterministic affine update separately to each pair preserves independence. Therefore the updated members are iid with the Gaussian law from step 3.1. By [A1] and [F4] that law is the exact filtering law at the fixed data.
The initialization in step 1.1 is the base case, and step 4.1 proves the claim at time from the induction hypothesis at time . Induction therefore gives the asserted iid exact filtering law for every .
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Sources
- Jan Mandel, Loren Cobb, and Jonathan D. Beezley, On the Convergence of the Ensemble Kalman Filter, §3 (standard reference, not scraped)
- K. J. H. Law, A. M. Stuart, and K. C. Zygalakis, Data Assimilation: A Mathematical Introduction, Chapter 4 §4.2.3 (standard reference, not scraped)