Application and validation of polynomial chaos methods to quantify uncertainties in simulating the Gulf of Mexico circulation using HYCOM.

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Application and validation of polynomial chaos methods to quantify uncertainties in simulating the Gulf of Mexico circulation using HYCOM. Mohamed Iskandarani Matthieu Le Hénaff Carlisle Thacker University of Miami Guotu Li Omar Knio Duke University Ashwanth Srinivasan Tendral LLC June 2, 2015

Outline Use Polynomial Chaos (PC) expansions to quantify uncertainties in oceanic forecasts Approximate model with an accurate surrogate Compute series coefficients via an ensemble Validate the accuracy of the surrogate Mine the series for statistical information in lieu of model Initial Condition uncertainties in the Gulf of Mexico How to perturb a field? How to localize perturbations around a dynamical process? Series Validation Statistical Outputs Uncertainty Experiments to date Initial conditions uncertainties (small ensemble) Initial conditions and wind forcing uncertainties

HYCOM surrogate idea M(x, t, ξ) is a model output ξ is a stochastic variable that represents the dependence of M on the uncertain input data ξ is characterized by its probability density function ρ(ξ) The mean of M is: M(x, t) = M(x, t, ξ) ρ(ξ) dξ Its variance is σ 2 (M) = (M M) 2 = (M M) 2 ρ(ξ) dξ A surrogate embodies the dependence of M on the uncertain data ξ via a spectral series in ξ: P M(x, t, ξ) = M n (x, t) ψ n (ξ) n=0

PC surrogate series M(x, t, ξ) = P n=0 M n (x, t) ψ n (ξ) Mn (x, t): series coefficients ψ k (ξ): orthonormal basis functions w.r.t. ρ(ξ) ψ m ψ n = ψ m (ξ)ψ n (ξ)ρ(ξ)dξ = δ m,n ψ m (ξ) consits of Legendre polynomials when ρ(ξ) is a uniform distribution mean: M = P n=0 M n (x, t)ψ n, ψ 0 = M 0 (x, t) Variance: (M M) 2 = P n=1 M 2 n (x, t) Where to truncate the series, P? Monitor Variance How to determine the coefficients M n?

Calculating the PC series coefficients Minimize the norm of the approximation error by using either Galerkin projection, interpolation, least square, or compressed sensing. All can be implemented via ensemble. The least square approaches are useful when model response includes model noise. Galerkin projection exploits orthogonality M = Mψ m = M(x, t, ξ)ψ m (ξ)ρ(ξ)dξ Q M(x, t, ξ q )ψ m (ξ q )ω q q=1 ξ q, ω q are appropriate quadrature roots,weights M(x, t, ξ q ) requires an ensemble at the quadrature roots

Gulf of Mexico Circulation Figure: Sea Surface Height in cm from AVISO Target Loop Current Eddy separation during May-June 2010. Capture the role of the frontal anticyclones in eddy detachment.

Uncertainty in Initial Boundary Conditions Computational challenge: Number of sample grows exponentially with the number of stochastic variables. Rely on EOFs to characterize uncertainty and reduce the number of stochastic variables. For 2 EOFs mode we have: [ M(x, 0, ξ 1, ξ 2 ) = M(x, 0) + λ1 M 1 ξ 1 + ] λ 2 M 2 ξ 2 (1) (λ k, M k ): are eigenvalues/eigenvectors of covariance matrix obtained from free-run simulation M: unperturbed initial condition M(x, 0, ξ): Stochastic initial condition input ξ 1, ξ 2 are the amplitudes of the perturbations

Figure: First and Second SSH modes from a 14-day series. The 2 modes account for 50% of variance during these 14 days. Characterize local uncertainty: get perturbation from short, 14-day, simulation. Uncertainty dominated by Loop Current (LC) dynamics Mode 1 seems associated with a frontal eddy

Figure: Vertical slice along 26.4N showing Temperature perturbations. The first mode shows a strong 2.5 C cooling in the vicinity of the frontal cyclones. The warm perturbation around 90W is at the southern edge of a small anticylone NW of the LC.

PC representation (ξ 1, ξ 2 ) independent and uniformly distributed random variables PC basis: Legendre polynomials of max degree 6, P = 28 Ensemble of 49 realizations for Gauss-Legendre quadrature 1 0.5 ξ 2 0-0.5-1 -1-0.5 0 0.5 1 ξ 1 Figure: Quadrature/Sample points in ξ 1, ξ 2 space. Center black circle corresponds to unperturbed run, while blue circles correspond to largest negative and positive perturbations.

Col 1: SSH of realization (1,1) with weakest frontal eddy Col 2: SSH of unperturbed realization (4,4) has medium strength frontal eddy Col 3: SSH of realization (7,7) has strogest frontal eddy and earliest LC separation Col 4: Loop current edge in ensemble

SSH stddev (cm) grows in time with maximum in LC region

PC-error: ɛ 2 2 = q [η( x, t, ξ q) η PC ( x, t, ξ q )] 2 ω q SSH PC-errors (cm) grow in time with maxima in LC region On day 60 PC-error is about 38% of stddev

Figure: Variance Analysis:The majority of the variance in the deep part of the Eastern Gulf of Mexico can be attributed to the 1st EOF, while the second mode plays a secondary role, particularly during the time span when the series is reliable (< 40 days, x-axis tick marks interval is 5-days).

Figure: Predictability Limit:Spatial distribution of the ratio of the forecast standard deviation to climatology standard deviation for SSH (from AVISO). The magenta lines show areas where the ratio > 1.

Initial Conditions & Wind Forcing Uncertainties Focus on the following two Quantities of Interest (QoIs): Sea Surface Height (SSH) averaged over a square area near the loop current (LC) region: [ 86.04, 85.20 ] in longitude and [25.19, 26.23 ] in latitude Mixed Layer Depth (MLD) averaged over the DeepWater Horizon (DWH) region: [ 88.44, 88.28 ] in longitude and [28.68, 28.79 ] in latitude Figure: Field snapshots on day 30: (Top) SSH; (Bottom) MLD Our HYCOM simulations start from 05-01-2010 to 05-30-2010. Fig.7 on the left shows HYCOM results on the last day of simulation using unperturbed initial and wind forcing fields.

1st Order Sensitivity: α S S i = i cα 2 < Ψα, Ψα > 1 P i=1 c2 < Ψ i i, Ψ i > Variance Analysis Total Order Sensitivity: α S i cα 2 < Ψα, Ψα > T T i = P i=1 c2 < Ψ i i, Ψ i > 0.8 0.6 0.64 SSH 0.8 0.6 0.77 MLD Si 0.4 Si 0.4 0.2 0.15 0.01 0.01 0.00 0.02 0.00 0.00 0 1 2 3 4 5 6 7 8 ξ i 0.8 0.77 SSH 0.6 0.2 0 0.8 0.6 0.07 0.02 0.00 0.00 0.00 0.00 0.01 1 2 3 4 5 6 7 8 ξ i 0.84 MLD Ti 0.4 Ti 0.4 0.2 0 0.24 0.04 0.05 0.02 0.04 0.02 0.02 1 2 3 4 5 6 7 8 ξ i 0.2 0 0.10 0.03 0.03 0.02 0.11 0.02 0.03 1 2 3 4 5 6 7 8 ξ i 1 0.91 1 0.88 S 0.5 S 0.5 0 0.04 0.05 Initial Condition Wind Forcing Interaction 0 0.05 0.08 Initial Condition Wind Forcing Interaction Figure: Sensitivities: (Top) 1st Order; (Middle) total Order; (Bottom) Initial and Wind forcing sensitivities.

Introduction Polynomial Chaos Primer UQ-Initial Conditions Perturbations The PC-Ensemble SSH: Joint Sensitivity (a) Interaction (b) Initial Condition (c) Wind Forcing

Introduction Polynomial Chaos Primer UQ-Initial Conditions Perturbations The PC-Ensemble MLD: Joint Sensitivity (d) Interaction (e) Initial Condition (f) Wind Forcing

Conclusions Polynomial Chaos are a promising approach in analyzing oceanic uncertainties It can monitor representation fidelity and adequacy of sampling The 14-day time series EOF analysis helped in designing perturbations focused on a Loop Current separation event. The PC-Series performs reasonably well in the 20 40 days range Predictability in SSH lost after about 20 days It is probably enough to perturb only the 2 leading EOF modes Including more uncertainty sources is more important for the current experiment than including more modes. SSH uncertainty due mainly to initial conditions except in shelf areas MLD uncertainty mainly caused by winds

Publications A. Srinivasan, J. Helgers, C. B. Paris, M. LeHenaff, H. Kang, V. Kourafalou, M. Iskandarani, W. C. Thacker, J. P. Zysman, N. F. Tsinoremas, and O. M. Knio. Many task computing for modeling the fate of oil discharged from the deep water horizon well blowout. In Many-Task Computing on Grids and Supercomputers (MTAGS), 2010 IEEE Workshop on, pages 1 7, November, 2010. IEEE. W. C. Thacker, A. Srinivasan, M. Iskandarani, O. M. Knio, and M. Le Henaff. Propagating oceanographic uncertainties using the method of polynomial chaos expansion. Ocean Modelling, 43 44, pp 52 63, 2012. A. Alexanderian, J. Winokur, I. Sraj, M. Iskandarani, A. Srinivasan, W. C. Thacker, and O. M. Knio, Global sensitivity analysis in an ocean general circulation model: a sparse spectral projection approach, Computational Geosciences, 16, 757 778, 2012. I. Sraj, M. Iskandarani, A. Srinivasan, W. C. Thacker, A. Alexanderian, C. Lee and S. S. Chen and O. M. Knio, Bayesian Inference of Drag Parameters Using AXBT Data from Typhoon Fanapi, Monthly Weather Review, 141, Issue 7, pp. 2347-2367, 2013. J. Winokur, P. Conrad, I. Sraj, O. M. Knio, A. Srinivasan, W. Carlisle Thacker, Y. Marzouk, and M. Iskandarani, A Priori Testing of Sparse Adaptive Polynomial Chaos Expansions Using an Ocean General Circulation Model Database, Computational Geosciences, 17, No 6, pp 899 911, 2013. I. Sraj, M. Iskandarani, A. Srinivasan, W. C. Thacker and O. M. Knio, Drag Parameter Estimation using Gradients and Hessian from a Polynomial Chaos Model Surrogate Monthly Weather Review, 142, No 2, pp 933941, 2013.