EnKF and Catastrophic filter divergence
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1 EnKF and Catastrophic filter divergence David Kelly Kody Law Andrew Stuart Mathematics Department University of North Carolina Chapel Hill NC bkelly.com June 4, 2014 SIAM UQ 2014 Savannah. David Kelly (UNC Catastrophic EnKF June 4, / 19
2 Talk outline 1. What is EnKF? 2. What is known about EnKF? 3. How can we use stochastic analysis to better understand EnKF? David Kelly (UNC Catastrophic EnKF June 4, / 19
3 The filtering problem We have a deterministic model dv = F (v with v 0 N(m 0, C 0. We will denote v(t = Ψ t (v 0. Think of this as very high dimensional and nonlinear. We want to estimate v = v(h for some h > 0 and = 0, 1,..., J given the observations y = Hv + ξ for ξ iid N(0, Γ. David Kelly (UNC Catastrophic EnKF June 4, / 19
4 We can use EnKF to draw approximate samples from the posterior. David Kelly (UNC Catastrophic EnKF June 4, / 19
5 The set-up for EnKF Suppose we are given the ensemble {u (1,..., u (K } at time. For each ensemble member, we create an artificial observation y (k +1 = y +1 + ξ (k +1, ξ (k +1 iid N(0, Γ. We update each member using the Kalman update ( u (k +1 = Ψ h(u (k + G(u y (k +1 HΨ h(u (k, where G(u is the Kalman gain computed using the forecasted ensemble covariance Ĉ +1 = 1 K K (Ψ h (u (k Ψ h (u T (Ψ h (u (k Ψ h (u. k=1 David Kelly (UNC Catastrophic EnKF June 4, / 19
6 There aren t many theorems about EnKF. Ideally, we would like a theorem about long time behaviour of the filter for a finite ensemble size. David Kelly (UNC Catastrophic EnKF June 4, / 19
7 Filter divergence In certain situations, it has been observed ( that the ensemble can blow-up (ie. reach machine-infinity in finite time, even when the model has nice bounded solutions. This is known as catastrophic filter divergence. We would like to investigate whether this has a dynamical ustification or if it is simply a numerical artefact. Harlim, Mada (2010, Gottwald (2011, Gottwald, Mada (2013. David Kelly (UNC Catastrophic EnKF June 4, / 19
8 Assumptions on the dynamics We make a dissipativity assumption on the model. Namely that dv + Av + B(v, v = f with A linear elliptic and B bilinear, satisfying certain estimates and symmetries. This guarantees uniformly bounded solutions. Eg. 2d-Navier-Stokes, Lorenz-63, Lorenz-96. David Kelly (UNC Catastrophic EnKF June 4, / 19
9 Discrete time results Let e (k = u (k v. For a fixed observation frequency h > 0 Theorem (AS,DK,KL If H = Id and Γ = γ 2 Id then there exists constant β > 0 such that ( E e (k 2 e 2βh E e (k e Kγ 2 2βh 1 e 2βh 1 So no finite time blow-up. David Kelly (UNC Catastrophic EnKF June 4, / 19
10 Discrete time results with variance inflation Suppose we replace Ĉ +1 α 2 I + Ĉ+1 at each update step. This is known as additive variance inflation. Theorem (AS,DK,KL If H = Id and Γ = γ 2 Id then there exists constant β > 0 such that ( E e (k 2 θ E e (k 1 θ Kγ 2 1 θ where θ = γ2 e 2βh α 2 +γ 2. In particular, if we pick α large enough (so that θ < 1 then lim E e(k 2 2Kγ2 1 θ David Kelly (UNC Catastrophic EnKF June 4, / 19
11 For observations with h 1, we need another approach. David Kelly (UNC Catastrophic EnKF June 4, / 19
12 The EnKF equations look like a discretization Recall the ensemble update equation ( u (k +1 = Ψ h(u (k + G(u y (k +1 HΨ h(u (k ( = Ψ h (u (k + Ĉ+1H T (H T Ĉ +1 H + Γ 1 y (k +1 HΨ h(u (k Subtract u (k from both sides and divide by h u (k +1 u(k h = Ψ h(u (k u (k h ( + Ĉ+1H T (hh T Ĉ +1 H + hγ 1 y (k +1 HΨ h(u (k Clearly we need to rescale the noise (ie. Γ. David Kelly (UNC Catastrophic EnKF June 4, / 19
13 Continuous-time limit If we set Γ = h 1 Γ 0 and substitute y (k +1, we obtain u (k +1 u(k h But we know that and Ĉ +1 = 1 K = 1 K = Ψ h(u (k u (k h + Ĉ+1H T (hh T Ĉ +1 H + Γ 0 1 ( Hv + h 1/2 Γ 1/2 0 ξ +1 + h 1/2 Γ 1/2 0 ξ (k +1 HΨ h(u (k Ψ h (u (k = u (k + O(h K (Ψ h (u (k Ψ h (u T (Ψ h (u (k Ψ h (u k=1 K (u (k k=1 u T (u (k u + O(h = C(u + O(h David Kelly (UNC Catastrophic EnKF June 4, / 19
14 Continuous-time limit We end up with u (k +1 u(k h = Ψ h(u (k u (k h + C(u H T Γ 1 0 C(u H T Γ 1 ( h 1/2 ξ +1 + h 1/2 ξ (k +1 This looks like a numerical scheme for Itô S(PDE 0 H(u(k v + O(h du (k = F (u (k C(uH T Γ 1 0 H(u(k v ( ( dw (k + C(uH T Γ 1/2 0 + db. David Kelly (UNC Catastrophic EnKF June 4, / 19
15 Nudging du (k = F (u (k C(uH T Γ 1 0 H(u(k v ( ( dw (k + C(uH T Γ 1/2 0 + db. 1 - Extra dissipation term only sees differences in observed space 2 - Extra dissipation only occurs in the space spanned by ensemble David Kelly (UNC Catastrophic EnKF June 4, / 19
16 Kalman-Bucy limit If F were linear and we write m(t = 1 K K k=1 u(k (t then dm = F (m C(uHT Γ 1 0 H(m v + C(uH T Γ 1/2 db 0 + O(K 1/2. This is the equation for the Kalman-Bucy filter, with empirical covariance C(u. The remainder O(K 1/2 can be thought of as a sampling error. David Kelly (UNC Catastrophic EnKF June 4, / 19
17 Continuous-time results Theorem (AS,DK,KL Suppose that {u (k } K k=1 satisfy ( with H = Id and Γ = γ2 Id. Let e (k = u (k v. Then there exists constant β > 0 such that 1 K K E e (k (t 2 k=1 ( 1 K K E e (k (0 2 exp (βt. k=1 David Kelly (UNC Catastrophic EnKF June 4, / 19
18 Why do we need H = Id and Γ = γ 2 Id? In the equation du (k = F (u (k C(uH T Γ 1 0 H(u(k v ( dw (k + C(uH T Γ 1/2 0 + db. The energy pumped in by the noise must be balanced by contraction of (u (k v. So the operator must be positive-definite. C(uH T Γ 1 0 H Both C(u and H T Γ 1 0 H are pos-def, but this doesn t guarantee the same for the product! David Kelly (UNC Catastrophic EnKF June 4, / 19
19 Summary + Future Work (1 Writing down an SDE/SPDE allows us to see the important quantities in the algorithm. (2 Does not prove that catastrophic filter divergence is a numerical phenomenon, but is a decent starting point. (1 Improve the condition on H. (2 If we can measure the important quantities, then we can test the performance during the algorithm. Well-posedness and accuracy of the ensemble Kalman filter in discrete and continuous time. D. Kelly, K.Law, A. Stuart. arxiv David Kelly (UNC Catastrophic EnKF June 4, / 19
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