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Stochastic modeling of mesoscale eddies in oceanic dynamics

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HAL Id: hal-02708167

https://hal.inria.fr/hal-02708167

Submitted on 1 Jun 2020

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Stochastic modeling of mesoscale eddies in oceanic dynamics

Long Li, Werner Bauer, Etienne Mémin

To cite this version:

Long Li, Werner Bauer, Etienne Mémin. Stochastic modeling of mesoscale eddies in oceanic dynamics.

Workshop on Frontiers of Uncertainty Quantification in Fluid Dynamics, Sep 2019, Pisa, Italy. �hal-

02708167�

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Stochastic modeling of mesoscale eddies in oceanic dynamics

Long Li

1

Werner Bauer

1

Etienne Mémin

1

1INRIA/IRMAR, Fluminance Group

Campus Universitaire de Beaulieu, F–35042 Rennes Cedex, France

Workshop on Frontiers of Uncertainty Quantification in Fluid Dynamics

Pisa(Italy), September 12, 2019

(3)

Motivations

Better small–scale representation : have explicit formulations and interpretations (v.s. parametrization with ad hoc tuning)

Physical consistency : respect a set of conservation laws (e.g. energy, circulation) (v.s. arbitrary Gaussian forcing)

Useful in uncertainty quantification (UQ) : provide more reliable

ensemble forecasts (EF) and more effiecient spread for ensemble data

assimilation (v.s. perturbations of initial condition (PIC) )

(4)

Outline

1

Location Uncertainty (LU) Principles

2

Stochastic Barotropic Vorticity Equation (SBVE)

3

Parametrizations of Noise

4

Long-term Diagnosis of Time–Statistics

5

Short-term Verification of Ensemble Forecasts

(5)

Location Uncertainty (LU) Principles

Stochastic flow :

dX

t

= w(X

t

, t)dt

| {z }

large–scale / resolved

+ σ(X

t

, t)dB

t

| {z }

small–scale / unresolved

Functional processs :

σ(x, t)dB

t

= Z

˘

σ(x, y, t)dB

t

(y)dy

B

t

is a cyclindrical Wiener process of infinite dimension (in some

Hilbert space) and σ ˘ is deterministic symmetric kernel

(6)

Location Uncertainty (LU) Principles

Covariance operator : Q(x, y, t, s) = E

h

σ(x, t)dB

t

σ(y, s)dB

s

T

i

= δ(t − s)dt Z

˘

σ(x, z, t) ˘ σ

T

(y, z, s)dz Variance tensor (per unit of time) :

a(x, t) = Q(x, t)

dt = σσ

T

(x, t) Turbulent Kinetic Energy (TKE) :

TKE = 1 2

tr(a) dt

(m

2·s−2)

(7)

Stochastic Reynolds Transport Theorem (SRTT)

We assume that ∇·σ = 0 in the following.

Rate of change of a scalar process θ within a volume transported by the stochastic flow :

d Z

V(t)

θ(x, t)dx = Z

V(t)

(D

t

θ + θ ∇· w

?

)dx

Stochastic transport operator : D

t

θ = d

4 t

θ + (w− 1

2 ∇· a

| {z }

w?

) ·∇ θdt + σdB

t

·∇ θ

| {z }

multiplicative noise

− ∇·( a 2 ∇θ)dt

| {z }

subgrid diffusion

w

?

: corrected drift – effect of statistical inhomogeneity of the small-scale flow component; generalization of the Stokes drift

[Bauer, Chandramouli, Chapron, Li & Mémin 2019a]

(8)

Conservation Laws

We assume that ∇·w

?

= 0 in the following.

Conservation of extensive scalar : D

t

θ = 0

Conservation of tracer energy :

[Resseguier, Memin & Chapron, 2017a]

d Z

1 2 θ

2

=

Z

θd

t

θ + 1 2 dhθi

t

= Z

1

2 θ

2

∇· (w

?

dt + σdB

t

)= 0 Energy decomposition of mean and variance fields :

0 = d dt

Z

1

2 ( E [θ])

2

+ d dt

Z

1

2 Var[θ]

(9)

Outline

1

Location Uncertainty (LU) Principles

2

Stochastic Barotropic Vorticity Equation (SBVE)

3

Parametrizations of Noise

4

Long-term Diagnosis of Time–Statistics

5

Short-term Verification of Ensemble Forecasts

(10)

Stochastic Barotropic Vorticity Equation (SBVE)

(11)

Stochastic Barotropic Vorticity Equation (SBVE)

Forced–dissipative advection of the potential vorticity (PV) q with source process :

D

t

q = (S

1

+ F + D)dt + S

2

dB

t

S

1

= 1 2

X

i,j=1,2

ij2

(∇

a

ij

· u), S

2

dB

t

= −tr

(σdB

t

)

T

∇u

T

Kinematic relationship between PV and stream function ψ : q = ∇

2

ψ + f, u = ∇

ψ

Conservation of kinetic energy in the absence of D and F :

[Bauer,

Chandramouli, Chapron, Li & Mémin 2019a]

d dt

Z

1

2 k∇ψk

2

= 0

(12)

Outline

1

Location Uncertainty (LU) Principles

2

Stochastic Barotropic Vorticity Equation (SBVE)

3

Parametrizations of Noise

4

Long-term Diagnosis of Time–Statistics

5

Short-term Verification of Ensemble Forecasts

(13)

Parametrizations of Noise

Homogeneous in space Stationary in time :

[Resseguier, Memin & Chapron, 2017b]

Homogeneous Non-stationary :

[Resseguier, Li, Jouan, Derian, Mémin & Chapron, 2019]

Based on estimation of the absolute diffusivity spectral density

(ADSD).

(14)

Parametrizations of Noise

Heterogeneous Stationary :

[Chandramouli, Mémin, Chapron & Heitz 2019b]

Based on snapshot proper orthogonal decomposition (POD) method

from data

(15)

Parametrizations of Noise

Heterogeneous Non-stationary

[Li, Bauer, & Mémin 2019]

: On-line learning

’Pseudo-observations’ from effective resolution

(16)

Outline

1

Location Uncertainty (LU) Principles

2

Stochastic Barotropic Vorticity Equation (SBVE)

3

Parametrizations of Noise

4

Long-term Diagnosis of Time–Statistics

5

Short-term Verification of Ensemble Forecasts

(17)

Long-term Diagnosis of Time–Statistics

Results predicted by DNS simulation :

(18)

Long-term Diagnosis of Time–Statistics

(19)

Long-term Diagnosis of Time–Statistics

(20)

Long-term Diagnosis of Time–Statistics

(21)

Long-term Diagnosis of Time–Statistics

(22)

Outline

1

Location Uncertainty (LU) Principles

2

Stochastic Barotropic Vorticity Equation (SBVE)

3

Parametrizations of Noise

4

Long-term Diagnosis of Time–Statistics

5

Short-term Verification of Ensemble Forecasts

(23)

Short-term Verification of Ensemble Forecasts

Observed samples are the filtered DNS PV at each grid point; Ensemble simulations are

performed with 30 particles from

t= 0

to

t= 30, starting from the (perturbed) filtered

DNS.

(24)

Ensemble Spreads

(25)

Reliability of Ensemble Forecasts

Rank histogram

( How well does the ensemble spread of the forecast represent the true uncertainty of the observations )

Flat : ensemble represent well the observed probability distribution;

U-shaped : ensemble spread too small, many observations falling outside the extremes of the ensemble;

Dome-shaped : ensemble spread too large, most observations falling near the center of the ensemble;

Asymmetric : ensemble contains bias.

(26)

Reliability of Ensemble Forecasts

(27)

Reliability of Ensemble Forecasts

The mean squared error (MSE) of the ensemble mean forecasts is identical to the average intra-ensemble sample variance (VAR), multiplied by an ensemble-size

N

– dependent inflation factor :

(qo−Eˆ[q])2

x

= N+ 1 N

Var[q]ˆ

x

0 5 10 15 20 25 30

-1 0 1 2 3 4 5 6 7

10-3

Other UQ metrics

[Resseguier, Li, Jouan, Derian, Mémin & Chapron, 2019]

: Continuous ranked

probability score (CRPS), Energy score, Variogram score.

(28)

Conclusions

Better eddy representation based on stochastic tranport;

Capture better on a coarse mesh the correct long-term time-statistics;

Spread is more accurate compared to PIC.

Work on ...

Strong interest in ensemble data assimilation with particle filter coupled

with LU.

(29)

Thanks for Your Attention!

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